Presentation type:
CR – Cryospheric Sciences

EGU26-2271 | Orals | MAL23-CR | Highlight | Julia and Johannes Weertman Medal Lecture

Of Known Unknowns and Unobserved Knowns 

Olaf Eisen

Two centuries ago, the pioneers of modern empirical research revolutionized Earth science by treating nature as a dynamic, interconnected system—one best understood not through hypotheses alone, but through systematic observation and measurement. "Nature does not answer questions we have not yet asked," as Alexander von Humboldt observed, "it shows us phenomena we must first learn to see as questions."

Yet science today often prioritizes hypothesis-driven research, leaving little room for the unexpected. This lecture explores the tension between discovery and prediction in glaciology, where some of the transformations have emerged not from testing hypotheses, but from exploration, curiosity, and serendipity.

From overlooked data to phenomena no one anticipated, glaciology’s future depends on our willingness to reclaim discovery science—not as a replacement for hypothesis testing, but as its essential counterpart. As Aldous Huxley reminds us, "There are things known and things unknown, and in between are the doors of perception." To address todays and future challenges in Earth science, we must keep those doors open.

 

How to cite: Eisen, O.: Of Known Unknowns and Unobserved Knowns, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2271, https://doi.org/10.5194/egusphere-egu26-2271, 2026.

EGU26-3134 | ECS | Orals | MAL23-CR | Highlight | Arne Richter Award for Outstanding ECS Lecture

Ice shelves, the Southern Ocean, and the future 

Kaitlin Naughten

Ice shelves, the floating extensions of the Antarctic Ice Sheet, are melted from below by the ocean. Increased ice shelf basal melting is the main mechanism by which Antarctica currently contributes to global sea level rise. As melt rates are sensitive to temperature, salinity, and circulation in tiny pockets of the Southern Ocean, predicting how they might respond to climate change is not straightforward. Projecting future ice shelf melting is at the forefront of coupled Earth system modelling, as most climate and ocean models still do not include ice shelves at all. This talk will summarise my research since 2020 on the future of ice shelf basal melting, focusing on three regions of Antarctica. In the Amundsen Sea, in West Antarctica, relatively warm ocean water already accesses the ice shelves. However, climate change is projected to make these regions warmer still, by increasing the volume of warm water flowing onshore. In contrast, Antarctica’s two largest ice shelves, the Ross and Filchner-Ronne, are currently bathed in cold water and melt rates are stable. However, numerous models predict that with sufficient climate change, these cavities could abruptly flip into a warm state similar to the Amundsen Sea. Sea level rise from Antarctica, therefore, is not all-or-nothing. Ice loss from some regions may already be committed, but in other regions abrupt changes may or may not be triggered, depending on how much the climate warms. Therefore, the trajectory of carbon emissions over the coming century will likely have a large impact on Antarctica’s long-term contribution to sea level rise.

How to cite: Naughten, K.: Ice shelves, the Southern Ocean, and the future, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3134, https://doi.org/10.5194/egusphere-egu26-3134, 2026.

EGU26-221 | ECS | Posters virtual | VPS20

Induced Diffusion of Interacting Internal Gravity Waves 

Yue Cynthia Wu and Yulin Pan

Induced diffusion (ID), an important mechanism of spectral energy transfer due to interacting internal gravity waves (IGWs), plays a significant role in driving turbulent dissipation in the ocean interior. In this study, we revisit the ID mechanism to elucidate its directionality and role in ocean mixing under varying IGW spectral forms, with particular attention to deviations from the standard Garrett-Munk spectrum. The original interpretation of ID as an action diffusion process, as proposed by McComas et al., suggests that ID is inherently bidirectional, with its direction governed by the vertical-wavenumber spectral slope σ of the IGW action spectrum, n ~ mσ. However, through the direct evaluation of the wave kinetic equation, we reveal a more complete depiction of ID, comprising both a diffusive and a scale-separated transfer rooted in the energy conservation within wave triads. Although the action diffusion may reverse direction depending on the sign of σ (i.e., red or blue spectra), the net transfer consistently leads to a forward energy cascade at the dissipation scale, contributing positively to turbulent dissipation. This supports the viewpoint of ID as a dissipative mechanism in physical oceanography. This study presents a physically grounded overview of ID and offers insights into the specific types of wave-wave interactions responsible for turbulent dissipation.

How to cite: Wu, Y. C. and Pan, Y.: Induced Diffusion of Interacting Internal Gravity Waves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-221, https://doi.org/10.5194/egusphere-egu26-221, 2026.

EGU26-1083 | ECS | Posters virtual | VPS20

Glacial lakes in permafrost terrain and downstream hazards 

Abhinav Alangadan and Ashim Sattar

A permafrost probability index (PPI) based on rock glacier inventory and machine learning models, including random forest, support vector machine, artificial neural network, and logistic regression, was generated for Kinnaur district, Himachal Pradesh, India. Intact rock glaciers were considered the dependent variable, and elevation, slope, aspect, and potential incoming solar radiation were used as independent variables to generate a spatially distributed, high-resolution permafrost probability index. Daily weather station data and daily multitemporal MODIS satellite data were used to train a linear regression model to predict the annual 0℃ isotherm in the region for the period of 2023-24, aiming to understand potential degradation by overlaying the isotherm on permafrost distribution. The random forest technique produced the best results with an overall accuracy of 89.43%. Seven glacial lakes were identified as located in potentially permafrost-degraded slopes, and the Kashang glacial lake was selected for detailed downstream glacial lake outburst flood process chain modeling based on its size, moraine-dammed proglacial setting, and potential downstream impact. The volume of the lake was estimated to be 8.6 × 106  m3 by extrapolating the contours from overdeepening of the main glacier. Three sources of avalanches were identified based on permafrost degradation and slopes greater than 30 degrees. Subsequently, three scenario-based process chains for glacial lake outburst floods were modeled. We simulate avalanche initialization, displacement wave generation, overtopping, moraine erosion, and downstream flooding. The modelling results revealed that the potential GLOF can cause a peak discharge of 16,167 ms⁻¹, and floodwater can reach the Kashang, where a hydropower is located, within 16 minutes  in the high-magnitude scenario. The findings can give important insights into GLOF hazard mitigation in the valley and can aid as preliminary data for various stakeholders working towards mitigating glacier-related hazards.

Keywords: Permafrost, GLOF, machine learning, r.avaflow, Himalaya

How to cite: Alangadan, A. and Sattar, A.: Glacial lakes in permafrost terrain and downstream hazards, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1083, https://doi.org/10.5194/egusphere-egu26-1083, 2026.

EGU26-3225 | ECS | Posters virtual | VPS20

Primary Factors Driving Extreme 2024 Early-spring Marine Heatwaves in the Tropical Atlantic: Shortwave Radiation and Mixed Layer Depth 

Jun-Chao Yang, Shenglong Li, Ingo Richter, Yi Liu, Yu Zhang, Ziguang Li, and Xiaopei Lin

The boreal early-spring of 2024 witnessed unprecedented marine heatwaves across the tropical Atlantic, setting a satellite-era record for basin-averaged marine heatwave intensity. Based on observational and reanalysis datasets and a mixed layer heat budget analysis, we identify three region-specific drivers. In the north (20°N–3°N), the event began in fall 2023 and was maintained by sustained positive shortwave radiation anomalies due to reduced cloudiness. Equatorial warming (3°N–3°S) was primarily driven by wind-driven ocean wave processes, amplified by a shallower mixed layer. In the south (3°S–20°S), the key mechanism was wind-driven mixed layer shoaling. The reduced cloudiness over the northern tropical Atlantic is linked to remote El Niño forcing, and the wind anomalies over the equatorial and southern tropical Atlantic are partly attributable to the concurrent South Atlantic Subtropical Dipole. Our findings clarify the multifaceted origins of such extreme marine heatwaves, offering crucial insights for improving their seasonal prediction.

How to cite: Yang, J.-C., Li, S., Richter, I., Liu, Y., Zhang, Y., Li, Z., and Lin, X.: Primary Factors Driving Extreme 2024 Early-spring Marine Heatwaves in the Tropical Atlantic: Shortwave Radiation and Mixed Layer Depth, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3225, https://doi.org/10.5194/egusphere-egu26-3225, 2026.

EGU26-3528 | Posters virtual | VPS20

Litter detection and mapping from the combined use of multispectral UAV imagery and Deep Learning: A case study from Greece 

Christina Mitsopoulou, George P. Petropoulos, Spyridon E. Detsikas, Christina Lekka, Konstantinos Grigoriadis, Vassilios Polychronos, Elisavet-Maria Mamagiannou, Christos Gkotsikas, Konstantinos Chardavellas, and Evina Katsou

Litter pollution has grown to be the most prominent threat to the coastal ecosystems, affecting both the environment and the local communities. An important step towards the mitigation of coastal pollution is the effective monitoring of the issue. The rapid evolution of Remote Sensing has offered many new techniques for the detection of beach litter, and Unmanned Aerial Vehicles (UAVs), especially, have proven to be invaluable tools. In this study, different approaches of beach litter detection are evaluated in order to determine which ones yield the most promising results. The data used were collected in the area of Palio Faliro, Greece and included RGB and Multi-spectral images. For the detection of the litter from the UAV images, two Deep Learning (DL) models were utilized, namely the Mask R-CNN and the YOLOv3. The accuracy of these two DL models in beach litter detection and also explore the potential challenges that may arise while trying to monitor the coastal environment with UAV methods. Our study findings suggest that the combined use of DL methods and UAV imagery can provide a cost-effective and scalable solution in litter detection and can assist relevant decision-making actions. Future work will focus on evaluating different DL methods under other experimental settings as well which will help towards assessing the wider applicability of the combined use of drone imagery and DL approaches in litter detection in coastal areas.

KEYWORDS: Remote Sensing, coastal little, UAVs, drones, deep learning, ACCELERATE project

Acknowledgements 

This study is financially supported by the ACCELERATE MSCA SE program of the European Union’s Horizon research and innovation program under grant agreement No. 101182930

How to cite: Mitsopoulou, C., Petropoulos, G. P., Detsikas, S. E., Lekka, C., Grigoriadis, K., Polychronos, V., Mamagiannou, E.-M., Gkotsikas, C., Chardavellas, K., and Katsou, E.: Litter detection and mapping from the combined use of multispectral UAV imagery and Deep Learning: A case study from Greece, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3528, https://doi.org/10.5194/egusphere-egu26-3528, 2026.

EGU26-3596 | ECS | Posters virtual | VPS20

Coastal Features Segmentation and Assessing their dynamics Using Machine Learning: Random Forest 

Prashant Kumar Makhan, Naresh Kumar Goud Lakku, Manasa Ranjan Behera, and Srineash Vijaya Kumar

Estuaries represent complex morphodynamic systems where interactions between tides, waves, and sediment processes control coastal stability and its ecological resilience. One such estuary, located along the bank of the Purna River in Navsari District, Gujarat, India, is currently experiencing severe erosion, with nearly two-thirds of the estuarine coastline affected.  Understanding spatio-temporal evolution of key coastal features is essential, including tidal flats, salt marshes, mangrove cover, and anthropogenic infrastructures within the study region. In this study, the coastal features segmentation is performed using the Random Forest on derived Landsat satellite imagery spectral indices spanning 2005–2024. The results indicate that over the past two decades, mangrove cover has increased by more than twofold, particularly near the estuary mouth. In contrast, tidal flat areas exhibited significant spatial variability, while salt marshes showed a considerable decline.

Shoreline change analysis shows extensive coastal erosion with the Net Shoreline Movement (NSM) exceeding 150 m in certain stretches, while the End Point Rate (EPR) ranged from 1.5 to 17 m/year (mean: 9.5 m/year). The analysis further indicates significant accretion in the estuaryward region and pronounced erosion along the seaward coast near its mouth. Further the coupled tide-wave numerical modelling was carried to attribute the observed changes. Overall, the findings highlight the complex interplay between natural coastal processes and anthropogenic pressures in this dynamic estuarine coastal system and provide valuable baseline information for coastal zone management and conservation planning.

Keywords: Estuary Dynamics, Random Forest, Shoreline changes, Tide Modelling, Wave Modelling, Remote Sensing.

How to cite: Makhan, P. K., Goud Lakku, N. K., Behera, M. R., and Vijaya Kumar, S.: Coastal Features Segmentation and Assessing their dynamics Using Machine Learning: Random Forest, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3596, https://doi.org/10.5194/egusphere-egu26-3596, 2026.

EGU26-3616 | ECS | Posters virtual | VPS20

Hybrid spectral downscaling and climate-driven variability of multimodal wave systems in the Gulf of Panama 

Ruby Vallarino-Castillo, Gabriel Bellido, Laura Cagigal, Vicente Negro-Valdecantos, Jesús Portilla-Yandún, Fernando Méndez, and José A. A. Antolínez

The Gulf of Panama is a semi-enclosed tropical basin where coastal processes are driven by a multimodal wave climate with pronounced interannual-to-decadal variability (Vallarino-Castillo, 2026). Offshore wave conditions were characterized at three spectral locations near the Gulf entrance using GLOSWAC-5 spectral data (Portilla-Yandún and Bidlot, 2025), revealing dominant wave systems with distinct directional origins and seasonal variability. A persistent Southern Ocean swell dominates year-round from the south–southwest, while northerly wind-seas associated with the Panama Low-Level Jet prevail during the dry season (December–April). Their opposing directions lead to frequent crossing-sea conditions, particularly along the western Gulf entrance, where partial blocking by the Azuero Peninsula enhances directional spreading. In contrast, more exposed central-eastern locations exhibit consistently multimodal spectra, whereas sheltered eastern areas show reduced northerly wind-sea influence and narrower directional ranges. During the wet season (May–November), additional southerly swell components linked to subtropical trade winds and the Chocó Low-Level Jet reinforce low-frequency energy, while episodic North Pacific swell incursions further increase spectral complexity. Building on these offshore patterns, we analyze how wave systems transform as they propagate across the Gulf’s complex basin geometry.

To resolve coastal wave conditions efficiently, we applied a hybrid spectral downscaling framework across the Gulf. Remote swell was reconstructed using BinWaves (Cagigal et al., 2024), which disaggregates each offshore spectrum into frequency–direction bins and propagates them individually with SWAN, assuming linear wave superposition over the nearshore of the Gulf of Panama, such that nonlinear wave–wave interactions are neglected during propagation. Nearshore spectra are then reassembled using precomputed propagation coefficients that account for coastal geometry. Locally generated seas were reconstructed with HyXSeaSpec, which extracts dominant atmospheric modes via multivariate dimensionality reduction, projects SWAN spectra onto a reduced EOF/PCA space and learns the nonlinear mapping between atmospheric modes and spectral coefficients using radial basis functions (RBFs). During prediction, new wind fields are projected into the reduced space to recover full directional spectra through inverse transforms. The hybrid workflow generates a 3-hourly directional wave spectrum hindcast (1969–2023) that combines remote swell and locally generated wind-sea contributions throughout the basin.

The ongoing nearshore analysis uses the reconstructed spectra to identify dominant variability patterns and coherent wave regimes, assessing how energy is redistributed within the gulf and how nearshore conditions respond to seasonal and interannual atmospheric forcing.

References:

Vallarino-Castillo R, Antolínez JAA, Negro-Valdecantos V, Portilla-Yandún J (2026). “Beyond understanding the role of far-field climate in the Gulf of Panama coastal dynamics: an analysis of long-term and seasonal variability of wave systems”. Climate Dynamics. https://doi.org/10.1007/s00382-025-08007-w

Portilla-Yandún J, Bidlot J-R (2025). “A global ocean spectral wave climate based on ERA-5 data: GLOSWAC-5”. Journal of Geophysical Research: Oceans. https://doi.org/10.1029/2025JC022629

Cagigal, L., Méndez, F.J., Ricondo, A., Gutiérrez-Barceló, D. & Bosserelle, C. (2024). “BinWaves: An additive hybrid method to downscale directional wave spectra to near-shore areas” en Ocean Modelling. 84, 102346.

How to cite: Vallarino-Castillo, R., Bellido, G., Cagigal, L., Negro-Valdecantos, V., Portilla-Yandún, J., Méndez, F., and A. A. Antolínez, J.: Hybrid spectral downscaling and climate-driven variability of multimodal wave systems in the Gulf of Panama, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3616, https://doi.org/10.5194/egusphere-egu26-3616, 2026.

             The variability in the circulation of the Northern Ionian Gyre (NIG) during 1988-2020 is assessed via dynamic-height fields in the upper layer (0-120 m and 0-398 m) derived from the monthly-averaged temperature and salinity fields of the Copernicus reanalysis data. The yearly-averaged dynamic-height fields agree with the corresponding fields of altimetric sea-surface topography used in previous studies that found, at the area of the NIG, a maximum-variability mode in the sea-surface topography of the Ionian Sea. In the present results, the NIG coincides with the area of a) the variability maxima of the dynamic-heights, existing on the standard-deviation (std) maps of the yearly-averaged dynamic heights during 1988-2020, b) the std maxima of the averaged density in the upper layer and c) the std maxima of the averaged salinity in the upper layer; the density-salinity correlation coefficients in the upper-layer within the NIG range from 0.87 to 0.74.

            Moreover, the std maxima of the precipitation fluxes, which have the dominant role on the evaporation-minus-precipitation (E-P) budget, are also located on the NIG area.   The 5-year running-averaged values of yearly E-P and salinity in the upper-layer of the NIG, which filter out the variability in less that ~5-6 years while they preserve the dominant variability in the periodicities (~8-10 years) of the NIG-circulation, have statistically significant correlations ranging from 0.53 for the period 1990-2018 to 0.73 for the period 1997-2018. After ~2005, the two timeseries resemble to each other even more.  In the upper layer, the area to the east-southeast of the NIG has statistically significant correlations in salinity (correlation coefficients: ~0.68-0.8) with the NIG area. This area can feed its higher-salinity signal to the NIG via northward transfer during the cyclonic circulation mode of the NIG.

How to cite: Kontoyiannis, H., Tsiaras, K., Iona, A., and Ballas, D.: The role of the air-sea water fluxes and the lateral influence on salinity in the bimodal circulation variability of the Northern Ionian Gyre in the period 1988-2020, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5203, https://doi.org/10.5194/egusphere-egu26-5203, 2026.

The Karakoram is known for its numerous surge glaciers and associated hazards from ice-dammed lake outburst floods. However, significant discrepancies persist in our understanding of surge trends and flood frequency. Therefore, this study aims to clarify the surge behaviour and related glacial lake outburst flood (GLOF) history for the Kumdan group of glaciers (Chong Kumdan, Kichik Kumdan, and Aktash). The study analysed historical archives, high-resolution satellite imagery, elevation changes derived from digital elevation models (DEMs), and glacier surface velocity from the ITS_LIVE dataset. Based on an in-depth review of historical records and cross-verified with multi-temporal satellite imagery, 16 GLOFs have been documented from this group since 1835, primarily originating from Chong Kumdan and Kichik Kumdan. The Aktash Glacier has surged several times but has not formed any ice-dammed lake due to efficient subglacial drainage, which prevents river blockages. Chong Kumdan and Aktash glaciers exhibit longer active phases (~7-10 years), whereas Kichik Kumdan Glacier shows shorter phases (~2 years). Out of all three Kumdan glaciers, the Chong Kumdan has produced the most devastating floods in 1835, 1926 and 1929. This glacier comprises two tributaries (a and b) and main trunk. Tributary ‘a’ follows a ~77-year surge cycle, and tributary ‘b’ and the main trunk exhibit asynchronous surge records. The surge cycle duration of Kichik Kumdan Glacier decreased from 33 years (1833–1866) to 27 years (1970–1997) due to climate warming. The last GLOFs from Chong Kumdan and Kichik Kumdan occurred in 1934 and 1903, respectively. DEM analysis from 2015 to 2022 reveals thickening in the reservoir areas of Chong Kumdan (~22 m) and Kichik Kumdan (~20 m), suggesting potential future surge but with a low probability of GLOF events. Overall, our study observed a decline in surge-generated GLOFs due to climate warming, reduced mass accumulation and weakening of ice dams. These insights will help downstream communities and risk management authorities better understand future risks and develop effective mitigation strategies.

How to cite: Halder, S. and Bhambri, R.: Impact of climatic warming on glacier surges and associated ice-dammed lake outburst floods in the Eastern Karakoram, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5669, https://doi.org/10.5194/egusphere-egu26-5669, 2026.

EGU26-8164 | Posters virtual | VPS20

Development of a Fine-Scale (1/648°) Nested Ocean Forecasting Model for the Tunisian Shelf 

Maher Bouzaiene and Milena Menna
A high-resolution forecasting nested hydrodynamic model has been developed for the Tunisian continental shelf to improve the representation of coastal circulation processes that are poorly resolved by basin-scale models. The fine-scale configuration employs a horizontal resolution of approximately 1/648° (~170 m) and is dynamically nested within a parent model of the central Mediterranean Sea. Initial and open boundary conditions are provided by the Mediterranean Sea Physics analysis at 1/24° resolution, while atmospheric forcing is derived from hourly GFS analysis data.
The enhanced spatial resolution enables a more realistic simulation of key coastal processes, including tidal dynamics, shelf currents, and nearshore circulation features. Model performance is evaluated against available in situ observations and Copernicus Marine Environment Monitoring Service (CMEMS) model products, demonstrating a substantial improvement in the representation of coastal hydrodynamics compared to lower-resolution configurations.
The developed forecasting modeling framework provides a robust tool for investigating physical processes on the Tunisian shelf and offers a valuable foundation for coastal management, environmental monitoring, and hazard assessment (e.g., storm surges and coastal flooding).

How to cite: Bouzaiene, M. and Menna, M.: Development of a Fine-Scale (1/648°) Nested Ocean Forecasting Model for the Tunisian Shelf, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8164, https://doi.org/10.5194/egusphere-egu26-8164, 2026.

EGU26-10227 | ECS | Posters virtual | VPS20

Analysis of the mechanisms underlying the low-frequency variability of the low-salinity tongue in the southeastern Indian Ocean 

pang yanran, qiwei sun, yuhong zhang, ying zhang, jianwei chi, and yan du

Ocean salinity serves as a key indicator of the global water cycle and exerts important controls on oceanic circulation, sea level, and stratification, thereby playing a critical role in marine thermodynamic and dynamic processes. In recent years, salinity variability in the tropical Indian Ocean, particularly its dynamic mechanisms and climatic effects, has attracted growing scientific interest. Using 31 years of satellite observations, in-situ data sets, and model reanalysis data, this study investigates the decadal variability and formation mechanisms of the low salinity tongue in the South Indian Ocean between the equator and 20°S. The results indicate that both the volume and mean salinity of the low-salinity tongue exhibit a quasi-12-year oscillation, which is primarily associated with the Interdecadal Pacific Oscillation (IPO). Further analysis reveals that on decadal timescales, variability in the volume of the upper 50 m low-salinity tongue is mainly driven by local precipitation. Through anomalous atmospheric circulation, sea surface temperature anomalies in the tropical Pacific lead to multi-year precipitation anomalies in the southeastern Indian Ocean, which subsequently alter the westward extension of the surface low-salinity tongue and ultimately govern its volume variability in the upper 50 m. However, in the subsurface layer (50 to 200 m), variability in the volume and average salinity of the low salinity tongue is dominated by freshwater transport associated with the Indonesian Throughflow (ITF). During negative IPO phases, wind anomalies over the tropical Pacific trigger oceanic wave adjustments, which enhance the ITF salinity transport. This process subsequently leads to an expansion of the low salinity tongue and a decrease in its average salinity in the southeastern Indian Ocean. Based on the three-dimensional variability of the low salinity tongue, this study reveals the relationships between the volume and average salinity of the tongue at different depths and local freshwater forcing, as well as salinity transport by the ITF, thereby contributing to an improved understanding of how regional water mass changes respond to long-term climate variability.

How to cite: yanran, P., sun, Q., zhang, Y., zhang, Y., chi, J., and du, Y.: Analysis of the mechanisms underlying the low-frequency variability of the low-salinity tongue in the southeastern Indian Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10227, https://doi.org/10.5194/egusphere-egu26-10227, 2026.

EGU26-10444 | Posters virtual | VPS20

Influence of Offshore Wind Farm Monopiles on Multi-Scale Hydrodynamics and Sediment Transport in a Wave-Current Environment 

Seyed Taleb Hosseini, Johannes Pein, Joanna Staneva, Emil Stanev, and Y. Joseph Zhang

The rapid expansion of offshore wind energy infrastructure represents a major anthropogenic modification of coastal and marginal seas, yet the physical interactions between monopile foundations, hydrodynamics, and sediment transport remain insufficiently quantified. This study investigates the impact of monopile foundations at the Meerwind offshore wind farm (German Bight, North Sea) on local and regional coastal dynamics. Using a high-resolution coupled wave-current-sediment transport model, we analyze hydrodynamic and sediment processes with mesh refinement of ~2 m near the structures to capture turbulent wake effects.

Our results demonstrate that monopile arrays act as significant sinks for wave energy: monthly mean significant wave heights (Hs) and mid-depth velocities decrease by ~5%, while turbulent kinetic energy increases by up to 70% near the foundations. Dominant westerly wind-driven waves modulate tidal asymmetry on the leeward (eastern) side of the piles, generating asymmetric turbulent wakes and altering bottom shear stress patterns.

Reduced wave-induced bottom stress enhances localized sediment deposition, increasing surface suspended sediment concentration (SSC) while reducing near-bottom loads. On a regional scale, wave attenuation leads to a ~1% decrease in depth-averaged SSC over a 20 km east of the piles. In consequence, the presence of the wind farm reduces the net inflowing sediment flux by ~25% within a 5 km radius during March 2020, linked to a ~2 cm attenuation of Hs.

These findings highlight how large-scale offshore energy infrastructure can reorganize sediment budgets and coastal morphodynamics under changing human activities, providing critical insights for the sustainable management of multi-use ocean spaces. Further work, including additional wind farms and extended simulation periods, is planned to substantiate these initial findings and better quantify cumulative impacts, particularly in light of ongoing erosion challenges in the Wadden Sea under sea-level rise.

How to cite: Hosseini, S. T., Pein, J., Staneva, J., Stanev, E., and Zhang, Y. J.: Influence of Offshore Wind Farm Monopiles on Multi-Scale Hydrodynamics and Sediment Transport in a Wave-Current Environment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10444, https://doi.org/10.5194/egusphere-egu26-10444, 2026.

EGU26-11166 | ECS | Posters virtual | VPS20

Improving coastal monitoring and forecasting systems through interoperable OGC API EDR-based data services 

Telmo Dias, Cesário Videira, Victor Lobo, Ana Cristina Costa, and Márcia Lourenço Baptista

Effective coastal monitoring and forecasting systems rely on the availability and timeliness of interoperable, standardized, and accessible marine data across observational, modelling and service layers. Fragmented data formats, legacy infrastructures, and non-standardized access mechanisms remain significant barriers to the seamless integration of ocean observations into operational monitoring and forecasting systems and downstream applications.

This study presents the development of a standards-based data workflow designed to enhance interoperability, scalability, and facilitate marine data integration, through the adoption of international standards and best practices. The proposed approach focuses on establishing robust data flows that transform, validate, and harmonize heterogeneous datasets (e.g., in situ near-real-time observations and numerical model outputs) into NetCDF format. Standardized and programmatic access to these datasets is enabled though the OGC API Environmental Data Retrieval protocol, implemented using the pygeoapi platform. By adopting open standards and service-oriented architectures, this framework enables efficient spatio-temporal querying of ocean variables, facilitating their assimilation into forecasting systems, decision-support tools, and customized applications. In parallel, geoportal interfaces were updated to integrate the new OGC API EDR services, ensuring that interoperable data access is available both through machine-to-machine interfaces and user-friendly graphical tools, supporting a broad range of user profiles and promoting citizen involvement and ocean literacy.

By addressing interoperability at the data, service, and user-interface levels, this work demonstrates how standardized data infrastructures are key enablers for improved, scalable, and sustainable coastal monitoring and forecasting capabilities.

How to cite: Dias, T., Videira, C., Lobo, V., Costa, A. C., and Lourenço Baptista, M.: Improving coastal monitoring and forecasting systems through interoperable OGC API EDR-based data services, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11166, https://doi.org/10.5194/egusphere-egu26-11166, 2026.

EGU26-11635 | ECS | Posters virtual | VPS20

Monitoring post-GLOF moraine dynamics at South Lhonak lake using satellite radars 

Utkarsh Verma and Ashim Sattar

The South Lhonak Lake (SLL) Glacial Lake Outburst Flood (GLOF) cascade event of 3-4 October 2023 triggered widespread devastation across Sikkim and the downstream region of Bangladesh, causing significant loss of lives and property. The post-disaster research shows that the GLOF event was triggered by a moraine failure, creating tsunami waves in the lake, eventually leading to the breach of the frontal moraine. Despite partial drainage of the lake in the 2023 event, the hazard potential of the lake needs further investigation. This makes it extremely important to continuously monitor the surrounding regions to identify unstable slopes that can potentially fail and impact the lake. The present study utilises a Sentinel-1 Small Baseline Subset (SBAS) workflow performed in the ASF OpenSARLab environment to analyse the condition of the moraines post-SLL disaster. Post-disaster analysis spanning October 2023 to September 2025 reveals continued moraine instability, characterised by an actively deforming zone along the right flank of the failed zone. This region shows a maximum LOS displacement rate of approximately -4 cm yr-1, with a maximum cumulative LOS displacement reaching around -6 cm in the ascending track and -5 cm in the descending track. The results indicate persistent post-failure deformation and ongoing slope instability in the moraines of South Lhonak. The study provides a critical insight into the temporal behaviour of moraine slopes. This study aimed at strengthening the disaster management strategies by integrating satellite-based deformation monitoring for early warning and risk reduction measures.

How to cite: Verma, U. and Sattar, A.: Monitoring post-GLOF moraine dynamics at South Lhonak lake using satellite radars, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11635, https://doi.org/10.5194/egusphere-egu26-11635, 2026.

EGU26-13664 | ECS | Posters virtual | VPS20

 Use of δ15N and macroalgae as indicators of the level of anthropogenic intervention in the Colombian Pacific. 

Ray Steven Arce-Sánchez, Diana Medina-Contreras, and Alberto Sánchez-González

Coastal ecosystems are highly vulnerable to nutrient-driven eutrophication from anthropogenic sources such as urbanization, wastewater discharge, and industrial development, among others, which alters their ecosystem services. In order to determine nitrogen sources, the nitrogen isotopic composition (δ15N) was analyzed in the macroalgae Boodleopsis verticillata and Bostrychia spp., collected between 2014 and 2016 at four localities with different degrees of anthropogenic disturbance: Valencia – Very Low Intervention (MBI-VA), Chucheros – Low Intervention (BAI-CHU), San Pedro – Moderate Intervention (MOI-SP), and Piangüita – High Intervention (ALI-PI) in the Colombian Pacific. The δ15N values ranged between 0.3 and 2.4‰ in MBI-VA, 1.8 and 3.4‰ in BAI-CHU, 2.3 and 5.5‰ in MOI-SP, and 2.3 and 10.16‰ in ALI-PI. Since the assumptions of normality and homogeneity of variances were not met (p < 0.05), a non-parametric Kruskal–Wallis test was applied, revealing significant differences in δ15N among localities (p < 0.0001). Dunn’s test indicated that MBI-VA and BAI-CHU differed significantly from MOI-SP and ALI-PI (p < 0.05). Three nitrogen sources were defined: atmospheric deposition, oceanic waters, and wastewater. Both species (B. verticillata andBostrychia spp.) showed a decreasing gradient of atmospheric deposition (87% ± 3% to 52% ± 7% and 82% ± 6% to 21% ± 11%, respectively) from MBI to ALI, in contrast to an increase in oceanic waters (8% ± 4% to 37% ± 13% and 12% ± 7% to 38% ± 21%) and wastewater contributions (5% ± 2% to 12% ± 6% and 7% ± 3% to 41% ± 12%). This pattern was more evident in Bostrychia spp., suggesting greater sensitivity to variations in nitrogen sources. Linear regression between δ15N and nitrate concentration yielded coefficients of determination of R2 = 0.71 for B. verticillata and R2 = 0.89for Bostrychia spp., indicating that isotopic variability was explained by nitrate. The potential of macroalgae as bioindicators of anthropogenic intervention in coastal ecosystems of the Colombian Pacific is suggested.

How to cite: Arce-Sánchez, R. S., Medina-Contreras, D., and Sánchez-González, A.:  Use of δ15N and macroalgae as indicators of the level of anthropogenic intervention in the Colombian Pacific., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13664, https://doi.org/10.5194/egusphere-egu26-13664, 2026.

EGU26-15143 | ECS | Posters virtual | VPS20

Holocene Sea Ice and Organic Matter Dynamics in the Southern Chukchi Sea Revealed by Lipid Biomarkers 

Kuang Jin, Anne de Vernal, Robert S. Pickart, Mickey Chen, Gerard Otiniano, and Trevor Porter

Arctic sea ice plays a critical role in regulating global climate and marine primary production, yet long-term records documenting its natural variability remain sparse in the Pacific sector of the Arctic Ocean. This limitation hampers our ability to establish a regionally coherent understanding of how sea ice responds to climatic and oceanographic forcing on centennial to millennial timescales. Here, we present a new biomarker-based reconstruction of Holocene sea ice and environmental change from the southern Chukchi Sea, north of the Bering Strait.

A 519-cm sediment core (SKQ-VC29) was recovered using a vibracorer and spans the last ~8.6 kyr, based on 17 AMS radiocarbon dates from shells and terrestrial macrofossils. Downcore concentrations of highly branched isoprenoids (HBIs) and sterols were quantified to reconstruct sea-ice conditions, marine productivity, and terrestrial organic matter (OM) inputs. Seasonal sea ice presence is inferred from IP25, a mono-unsaturated HBI produced by sea-ice diatoms, while open-water conditions and phytoplankton productivity are tracked using HBI III, brassicasterol, and dinosterol. These proxies are combined using the PIP25 index to provide a semi-quantitative reconstruction of sea-ice cover. Terrestrial inputs are assessed using vascular-plant sterols (campesterol and β-sitosterol), alongside bulk δ¹³C and C:N ratios.

The record indicates predominantly open-water conditions during the early to mid-Holocene, followed by the reappearance of seasonal sea ice at ~2.5 kyr BP—substantially later than in more northerly Arctic records. This delayed signal suggests that Neoglacial sea-ice expansion in the Pacific Arctic was spatially heterogeneous. Bulk OM proxies and declining β-sitosterol concentrations indicate a progressive reduction in terrestrial OM delivery through the Holocene, while marine productivity remains relatively stable. A pronounced shift at ~4 ka BP marks reduced organic carbon accumulation and broader environmental reorganization.

Together, these results improve spatial coverage of Holocene sea-ice reconstructions in the Pacific Arctic and highlight the complex, regionally variable nature of sea-ice evolution in a climatically sensitive gateway region.

How to cite: Jin, K., de Vernal, A., Pickart, R. S., Chen, M., Otiniano, G., and Porter, T.: Holocene Sea Ice and Organic Matter Dynamics in the Southern Chukchi Sea Revealed by Lipid Biomarkers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15143, https://doi.org/10.5194/egusphere-egu26-15143, 2026.

EGU26-16248 | Posters virtual | VPS20

Explainable Expert-in-the-loop sea-ice classification with statistical models 

Corneliu Octavian Dumitru, Chandrabail Karmakar, and Stefan Wiehle

Sea ice classification is often a crucial step to predict climatic insights and ensure safe marine navigation. In the last few decades, satellite information has been widely used to classify sea ice in broad areas for practical applications. However, common problems are:

1) Low resolution of satellite images to provide precise classification,

2) High computational need, and

3) Scarcity of general models to discover unknown patterns in the data, especially those that enable free selection of satellite sensors to fit the application at hand.

We propose an explainable unsupervised model to integrate ice-experts’ inputs to models so that the problem of having low-resolution data can be overcome. In other words, the results of the models, given as semantic maps, can be further refined using inputs from ice-experts.

Model explainability and visual interpretation of models serve as tools to talk to’ domain experts. The use of Explainable AI in such vital activities ensures trust and easy detection of error. We present an example from a sea ice classification with Sentinel-1 time-series in the scope of the Horizon 2020 project ExtremeEarth.

A further example from the Horizon Europe project dAIEdge demonstrates the use of these explainable models for ‘on-the-edge’ inference.

How to cite: Dumitru, C. O., Karmakar, C., and Wiehle, S.: Explainable Expert-in-the-loop sea-ice classification with statistical models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16248, https://doi.org/10.5194/egusphere-egu26-16248, 2026.

EGU26-16935 | Posters virtual | VPS20

Dust in the Arctic: feedbacks and interactions between climate change, aeolian dust and ecosystems 

Outi Meinander, Andreas Uppstu, Pavla Dagsson-Waldhauserova, Christine Groot-Zwaaftink, Christian Juncher Jørgensen, Alexander Baklanov, Adam Christenson, Andreas Massling, and Mikhail Sofiev

Dust in the Arctic is an emerging topic related to climate and environmental impacts. The United Nations (UN) General Assembles and the UN Coalition to Combat Desertification (UNCCD) have reiterated that the global frequency, intensity, and duration of Sand and Dust Storms (SDS) have increased in the last decade and that SDS have natural and human causes that can be exacerbated by desertification, land degradation, drought, biodiversity loss, and climate change. UNCCD and FAO have also highlighted that emerging SDS source areas have been associated with the warming of the Arctic and high latitude regions, the seasonal or permanent drying of inland waters and river deltas, or are following large-scale deforestation and wildfires, or even the ploughing of a single field. Loss of snow cover, retreat of glaciers, and increase in drought intensity due to climate change can lead to surface conditions that increase the likelihood of creation, continuation and expansion of SDS source areas.

Climatic feedback mechanisms and ecosystem impacts related to dust in the Arctic include direct radiative forcing (absorption and scattering), indirect radiative forcing (via clouds and cryosphere), semi-direct effects of dust on meteorological parameters, effects on atmospheric chemistry, as well as impacts on terrestrial, marine, freshwater, and cryosphere ecosystems. Here we give an overview of our recent understanding on dust emissions and their long-range transport routes, deposition, and ecosystem effects in the Arctic as presented in Meinander et al. (2025), part of the series of review papers of the Arctic Council Working Group AMAP (Arctic Monitoring and Assessment Program) and CAFF (Conservation of Arctic Flora and Fauna), where the target audience is the scientific community focusing on the Arctic. Additional audiences include policy advisers and other staff in environmental-related ministries.

We conclude that the multiple mechanisms related to dust emissions, transport and deposition both cool and warm the climate system, with an uncertain net effect. Dust plays a significant role in terrestrial and aquatic ecosystems, e.g., by providing nutrients, and with impacts on the availability of light and water. Due to Arctic warming, HLD dust emissions can be expected to increase. The contributions of LLD and HLD complicates the interpretation of how much different sources contribute to the dust loadings and corresponding temporal and spatial deposition patterns. Another challenge is that low latitude dust source emissions of road and agricultural dust is barely characterized.

Reference:

Meinander O, Uppstu A, Dagsson-Waldhauserova P, Groot Zwaaftink C, Juncher Jørgensen C, Baklanov A, Kristensson A, Massling A and Sofiev M (2025). Dust in the arctic: a brief review of feedbacks and interactions between climate change, aeolian dust and ecosystems. Front. Environ. Sci. Sec. Interdisciplinary Climate Studies, Volume 13 – 2025. doi: 10.3389/fenvs.2025.1536395. CAFF-special issue.

 

How to cite: Meinander, O., Uppstu, A., Dagsson-Waldhauserova, P., Groot-Zwaaftink, C., Juncher Jørgensen, C., Baklanov, A., Christenson, A., Massling, A., and Sofiev, M.: Dust in the Arctic: feedbacks and interactions between climate change, aeolian dust and ecosystems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16935, https://doi.org/10.5194/egusphere-egu26-16935, 2026.

Accelerated glacier retreat in the Western Himalaya has led to rapid expansion of glacial lakes and increasing concern over Glacial Lake Outburst Flood (GLOF) hazards. This study presents a basin-scale assessment of glacial lake evolution, potential future lake formation, and GLOF susceptibility in the Chenab Basin, integrating multi-temporal remote sensing, terrain analysis, and probabilistic exposure modelling. A decadal inventory of glacial lakes was developed for five time periods (1990, 2000, 2010, 2020 and 2025) using Landsat and Sentinel-2 imagery, combined with semi-automated extraction and geomorphological classification. Results reveal a consistent increase in both lake number and total area over the last three decades. Potential future glacial lakes were identified using various ice-thickness modeling approach applied to current glacier extents. This analysis presents an inventory of the future glacial lake in the entire basin giving special emphasis to determining the characteristics of the future lake including maximum extent of the future lakes and volume of the future glacial lakes. GLOF susceptibility of existing lakes was evaluated using a multi-criteria framework to identify critical lakes requiring priority monitoring. Downstream exposure was further assessed using the Monte Carlo Least Cost path approach, explicitly accounting for uncertainty in breach location and flood routing parameters to delineate probable impact corridors. The framework provides new insights into evolving cryospheric hazards in the Chenab Basin and demonstrates the utility of combining lake dynamics, future lake potential, susceptibility assessment, and probabilistic exposure analysis for improved GLOF risk prioritization in the Western Himalayas.

How to cite: Das, D. R. and Sattar, A.: Evolution of present and potential future glacial lakes and implications for GLOF hazard in the Chenab Basin, Western Himalaya, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17889, https://doi.org/10.5194/egusphere-egu26-17889, 2026.

EGU26-20743 | Posters virtual | VPS20

Machine Learning based Seasonal Streamflow Forecasting in Cold-Region Catchments: Insights from LamaH-Ice dataset 

Golda Prakasam, Mikko Strahlendorff, Anni Kröger, and Andri Gunnarsson

Machine learning (ML) remains one of the best approaches for long-term seasonal streamflow forecasting in cold regions owing to its capacity to capture nonlinearity between inputs and outputs, as well as its scalability across hydroclimatic regimes. ML’s main advantage lies in the generalizability of these models when applied to heavily glacierized catchments. In this data-driven study, we mainly utilize the Extreme Gradient Boosting (XGBoost) regression to train and test seasonal streamflow predictions using the LArge-SaMple DAta for Hydrology and Environmental Sciences for Iceland (LamaH-Ice). This new dataset for Iceland, published in 2024 consists of topographic, hydroclimatic, land cover, vegetation, soil, geological, and glaciological attributes that are essential for understanding cryosphere–hydrology processes in cold regions. For more than 100 basins, time series information on meteorological forcings and variables relevant to cold-region hydrology, such as MODIS (Moderate Resolution Imaging Spectroradiometer) snow cover, glacier albedo are also available. The majority of gauged rivers in LamaH-Ice are reported to have minimal human disturbances, making the dataset particularly unique. The XGBoost model demonstrates strong predictive skill across the study basins, as indicated by Kling-Gupta Efficiency (KGE) and Nash-Sutcliffe Efficiency (NSE) metrics exceeding 0.98. Ultimately high-precision streamflow forecasting is needed to track hydrometeorological hazards and to aid our ability to manage water resources in cold regions, which are a source for irrigation and hydropower.

References

Helgason, Hordur Bragi, and Bart Nijssen. “LamaH-Ice: LArge-SaMple DAta for Hydrology and Environmental Sciences for Iceland.” Earth System Science Data, vol. 16, no. 6, 13 June 2024, pp. 2741–2771, doi:10.5194/essd-16-2741-2024. 

Strahlendorff, Mikko, et al. “Forestry Climate Adaptation with HarvesterSeasons Service—a Gradient Boosting Model to Forecast Soil Water Index SWI from a Comprehensive Set of Predictors in Destination Earth.” Frontiers in Remote Sensing, vol. 5, 20 Dec. 2024, doi:10.3389/frsen.2024.1360572.

How to cite: Prakasam, G., Strahlendorff, M., Kröger, A., and Gunnarsson, A.: Machine Learning based Seasonal Streamflow Forecasting in Cold-Region Catchments: Insights from LamaH-Ice dataset, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20743, https://doi.org/10.5194/egusphere-egu26-20743, 2026.

EGU26-21809 | ECS | Posters virtual | VPS20

D-PERSEUS: A Drone Radar Mission to Study a Debris-Covered Glacier on Mars 

Reed Spurling, Stefano Nerozzi, and Roberto Aguilar

Near-surface water ice in Phlegra Montes, Mars, could support human exploration and settlement. Orbital sounding radar provides strong evidence for the existence of this ice, as does morphology consistent with debris-covered glaciers. Impact excavation of these glacier-like features has exposed ice, visible in HiRISE images, but the distribution and quantity of this ice is uncertain, necessitating further evaluation for its potential to support human exploration. We are developing the Prototype Radar Sounding Experiment for Unveiling the Subsurface (PERSEUS) instrument to study debris-covered glaciers on Earth and Mars, and we propose D-PERSEUS, a mission to study a debris-covered glacier in Phlegra Montes using a drone-based Ground Penetrating Radar like this one. This mission could verify the presence of water ice in-situ and improve characterization of water ice resources, which could serve as exploratory work ahead of a potential Mars Life Explorer mission.

How to cite: Spurling, R., Nerozzi, S., and Aguilar, R.: D-PERSEUS: A Drone Radar Mission to Study a Debris-Covered Glacier on Mars, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21809, https://doi.org/10.5194/egusphere-egu26-21809, 2026.

EGU26-22059 | ECS | Posters virtual | VPS20

Indirect assimilation of remote sensing reflectance: case study in the Liguria Sea 

Carlos Enmanuel Soto Lopez, Paolo Lazzari, Fabio Anselmi, and Anna Teruzzi

The dataset with the most spatial coverage for data assimilation of biogeochemical models in operational systems is the satellite-derived data. Nevertheless, variables derived from Remote Sensing Reflectance (RSR), like the sea surface chlorophyll concentration, for regions like coastal areas, can reach big errors if compared with in situ measurements. For this reason, a suggestion with the aim of improving the assimilated results comes from the direct assimilation of Remote Sensing Reflectance, removing the error derived from inferring the biogeochemical variable before assimilating. In this work, we focus on a case study, using the Biogeochemical Flux Model (BFM) merged with a hydrological model, we study the effects of the direct and indirect assimilation of RSR in a region located in the Ligurian Basin of the northwestern Mediterranean Sea.  For both assimilation experiments, the algorithm used was an Error Subspace Kalman Filter. To assess the results, we compared them with climatologies computed with in situ measurements, highlighting the advantages and disadvantages of both approaches. 

How to cite: Soto Lopez, C. E., Lazzari, P., Anselmi, F., and Teruzzi, A.: Indirect assimilation of remote sensing reflectance: case study in the Liguria Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22059, https://doi.org/10.5194/egusphere-egu26-22059, 2026.

CR1 – The State of the Cryosphere: Past, Present, Future

EGU26-176 | ECS | Posters on site | CR1.1

Low-Cost Terrestrial Photogrammetry System for Monitoring Calving from Lake-Terminating Glaciers 

Sayantan Mandal, Liam Taylor, Raaj Ramsankaran, and Duncan Quincey

In-situ monitoring of calving process from lake-terminating glaciers in the Himalayas remain scarce, despite being a significant component controlling glacier retreat. Acquiring in-situ measurements are challenging due to harsh terrain and extreme weather conditions, which has typically resulted in the use of expensive, state-of-the-art terrestrial observational systems. Such limitation in data acquiring leads to an incomplete understanding of calving-induced glacial mass loss and retreat. In this study, we evaluate the effectiveness of a low-cost Raspberry-Pi based terrestrial photogrammetry system for annual monitoring of calving from lake-terminating glaciers. We tested the proposed system for monitoring calving at lake-terminating Panchinala-B Glacier, Indian Western Himalayas. The photogrammetry system consists of an array of Raspberry-Pi powered time-lapse cameras, which took multi-view stereo images of the glacier front face over a 12-month period between August 2023 and August 2024. The images were processed in a Structure-from-Motion (SfM) workflow to generate two, annually separated, point clouds. The Multiscale Model-to-Model Cloud Comparison (M3C2) distance of the annually separated point clouds yielded a mean terminus position change (retreat) of 0.88 m, with a mean absolute error of (+/-) 5.8 m. Using the above obtained parameters a calving rate and calving mass flux of  16.3 (+/-) 4.29 m/annum and 0.00017 (+/-) 0.000125 Gt/annum respectively can be quantified. Further, numerous environmental and system design-based challenges were encountered, which affected the quality of the obtained calving estimates. These challenges were carefully understood, and we provide further recommendations for the future use of similar low-cost systems for long-term glacier monitoring, which demonstrate good  potential for characterising the magnitude and frequency of calving processes at lake-terminating glaciers.

How to cite: Mandal, S., Taylor, L., Ramsankaran, R., and Quincey, D.: Low-Cost Terrestrial Photogrammetry System for Monitoring Calving from Lake-Terminating Glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-176, https://doi.org/10.5194/egusphere-egu26-176, 2026.

EGU26-791 | Orals | CR1.1

 Melting Glaciers in the Western Himalaya: Evidence from In-Situ Seasonal and Annual Mass Balance Observations from the Ladakh Himalaya  

Shakil Ahmad Romshoo, Basharat Nabi Lone, Umar Ameen Shah, Mustaffa Bhat, Waseem Shah, Mudasir Bhat, Waheed Shah, Aazim Yousuf, Tariq Abdullah, Khalid Omar Murtaza, Gowhar Lone, Adil Mir, Ubair Shah, Omar Paul, and Shakil Romshoo

Field-based seasonal and annual mass-balance observations collected over the past one decade from four benchmark glaciers in the Ladakh region of the western Himalaya, Viz., Pensilungpa, Drang-Drung, Kangrez, and Machoi, indicate a consistent and significant loss of glacier mass across all elevation bands. Mass-balance estimates, obtained from stake networks and snow-pit observations exhibit persistently negative annual values, with enhanced ablation in lower and mid-elevation zones and limited accumulation at higher elevations. The average annual glacier mass balance ranges from −0.4 to −1.4 m w.e. yr⁻¹, with glacier-specific mass balance ranges of −0.8 to −1.4 m w.e. (Pensilungpa), −0.6 to −1.2 m w.e. (Drang-Drung), −0.5 to −1.1 m w.e. (Kangrez), and −0.4 to −0.9 m w.e. (Machoi). Winter accumulation across these four benchmark glaciers ranges from +0.3 to +1.1 m w.e., while summer ablation varies between −0.8 and −2.0 m w.e., reflecting strong altitude-dependent glacier-melt. All glaciers show steep mass-balance gradients, with a pronounced melt in lower ablation zones, and limited but persistent accumulation at higher elevations in the accumulation zones. Drang-Drung and Kangrez exhibit relatively stronger winter mass gains at higher elevations, while Pensilungpa and Machoi display the most intense summer ablation. Although the accumulation zones still gain seasonal mass, but it is not enough to offset the significant ablation as the ablation zones dominate glacier area, causing cumulative negative mass balances. The upward-shifted equilibrium-line altitudes and the dominance of ablation over accumulation indicate the increasing glacier sensitivity to regional warming in the cold desert Ladakh region.

Based on typical uncertainties associated with stake measurements, density sampling, and spatial interpolation of point observation, the uncertainty in annual mass-balance is estimated at ±0.25–0.40 m w.e. yr⁻¹. Despite this uncertainty, the results robustly demonstrate significant glacier mass loss in the  Ladakh region, underscoring enhanced cryospheric vulnerability to climate change and potential impacts on hydrological regimes in the upper Indus basin. These findings are consistent with regional trends in the Himalaya showing accelerated ice loss and rising ELAs, underscoring the growing sensitivity of cold-arid glaciers to climate warming, once considered relatively resilient. Continued mass loss has significant implications for water security, climate adaptation, and glacier hazard risk management across the upper Indus basin.

How to cite: Romshoo, S. A., Lone, B. N., Shah, U. A., Bhat, M., Shah, W., Bhat, M., Shah, W., Yousuf, A., Abdullah, T., Murtaza, K. O., Lone, G., Mir, A., Shah, U., Paul, O., and Romshoo, S.:  Melting Glaciers in the Western Himalaya: Evidence from In-Situ Seasonal and Annual Mass Balance Observations from the Ladakh Himalaya , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-791, https://doi.org/10.5194/egusphere-egu26-791, 2026.

EGU26-1391 | ECS | Orals | CR1.1 | Highlight

Large-Scale Detection of Alpine Glacier Crevasses Using Remote Sensing and Deep Learning 

Celia A. Baumhoer, Selina Straßburger, Sarah Leibrock, and Andreas Dietz

Knowledge of crevasse locations is essential for improving our understanding of glacier dynamics. In addition, accurate information on crevasses is crucial for mountaineering safety and enables reliable route planning. However, large-scale monitoring remains difficult because crevasses vary greatly in appearance and often show low contrast on snow-covered surfaces, limiting the effectiveness of traditional detection methods. Here, we present an automated crevasse-detection approach based on a multi-task neural network trained on high-resolution orthophotos of Austrian alpine glaciers.

The model was developed using 20 cm aerial imagery of glaciers in the Ötztal and Stubai Alps. Through systematic training and validation, the network achieved 86% detection accuracy across independent test sites, demonstrating robust performance in diverse glaciological settings. The multi-task architecture enables simultaneous feature extraction and classification, efficiently handling the complex spectral and textural characteristics of crevassed ice surfaces.

Following successful validation, we applied the method to all glaciated areas in Austria, producing a comprehensive, high-resolution dataset of crevasse locations. We analysed the spatial distribution of crevasses on Austrian glaciers in different mountain regions, including Hohe Tauern, Dachstein, Ötztal, Stubai, Silvretta and Zillertal.  Analysis of this dataset reveals spatial patterns of crevasse distribution and quantitative metrics on variations in crevasse density across slope, elevation, velocity, curvature and aspect.

The crevasse location dataset provides glacier modelers with detailed boundary conditions for glacier modelling and helps mountaineers plan safe routes. This dataset has already been incorporated into recently published hiking maps by the Austrian Alpine Club and demonstrates how machine learning and open data initiatives can bridge glaciological research and practical applications.

How to cite: Baumhoer, C. A., Straßburger, S., Leibrock, S., and Dietz, A.: Large-Scale Detection of Alpine Glacier Crevasses Using Remote Sensing and Deep Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1391, https://doi.org/10.5194/egusphere-egu26-1391, 2026.

EGU26-2248 | ECS | Posters on site | CR1.1

Uncertainty propagation from Sentinel-2A/B-derived velocity to glacier strain rates: a first-principles perspective 

Chentong Zhang, Xianwei Wang, and Yi Zhou

Satellite remote sensing has become a cornerstone for monitoring glacier surface velocity and strain rates, with normalized cross-correlation (NCC) techniques widely adopted due to their efficiency and robustness. However, current approaches to quantifying strain-rate uncertainty exhibit substantial limitations. They rely primarily on empirical statistics or classical error-propagation theory, which implicitly assumes spatially independent Gaussian velocity errors and fails to account for the numerical effects introduced by NCC algorithmic parameters and environmental conditions. As a result, strain-rate errors derived from NCC-based velocity fields are poorly characterised at sub-monthly timescales over rapidly evolving glaciers, and technical uncertainties cannot be effectively separated from systematic velocity-field mismatches, limiting the applicability of remote-sensing products in glacier dynamics studies.

 

We develop a first-principles uncertainty theory by explicitly modelling the fundamental error mechanisms underlying NCC-derived velocity measurements. Building upon the classical error-propagation framework, we combine ordinary differential equations and stochastic process theory to rigorously derive analytical error expressions for two commonly used strain-rate formulations applied to NCC-derived velocity fields: nominal strain rate and logarithmic strain rate. The theory demonstrates that, although the nominal strain-rate error shares a similar mathematical structure with classical error propagation, its coefficients are substantially smaller than those predicted by traditional formulations. In contrast, the logarithmic strain rate (based on the Nye model and Alley grid-based implementation) converges to the true strain rate under normal circumstances, while degenerating to the nominal strain-rate solution in the worst case.

 

We validate the theoretical predictions using Helheim Glacier, Greenland, as a test case. Surface velocities are extracted from 616 Sentinel-2A/B image pairs with time baselines from 1 to 32 days, followed by statistical analysis of strain-rate errors. Under controlled NCC failure rates, the theoretical model achieves a goodness of fit exceeding R > 0.8, confirming the robustness of the proposed framework.

 

Our results further reveal a strong dependence of strain-rate error on temporal baseline and pixel distinguishing capacity. For longer baselines (Δt > 18 days over Helheim Glacier), high-strain environments such as shear margins lead to a loss of image similarity, increasing NCC failure rates and inducing systematic velocity-field errors that cause strain-rate overestimation. For shorter baselines (Δt < 10 days), nominal strain rates are strongly limited by pixel distinguishing capacity, producing random non-zero velocity artefacts over stable terrain. Owing to the error attenuation behaviour of logarithmic strain rate, the effective lower bound of usable time baselines is reduced to approximately 3 days, enabling high-temporal-resolution monitoring. Based on the derived error equations, we propose a practical time-baseline selection guideline that constrains random strain-rate errors induced by technical uncertainty, while facilitating the separation of systematic velocity-field errors.

 

Overall, this work provides an end-to-end uncertainty quantification framework linking remote-sensing techniques to glacier strain-rate products, offering a theoretical foundation for quality control, uncertainty assessment, and data assimilation in next-generation glacier strain-rate monitoring.

How to cite: Zhang, C., Wang, X., and Zhou, Y.: Uncertainty propagation from Sentinel-2A/B-derived velocity to glacier strain rates: a first-principles perspective, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2248, https://doi.org/10.5194/egusphere-egu26-2248, 2026.

EGU26-2645 | ECS | Orals | CR1.1

Firn-Line Monitoring over the Juneau Icefield in Alaska Using SAR Data 

Kenshiro Arie and Takeo Tadono

The equilibrium-line altitude (ELA) is a key indicator of the climatic limit for glacier sustainability. Monitoring ELA is therefore essential for understanding and projecting glacier change. In practice, however, direct ELA measurements from field surveys (the glaciological method) are available for only a limited number of glaciers because sustained observations require substantial time and labor.

Here, we observe multi-decadal variations in firn-line altitude (FLA) over an Alaskan icefield located near a well-monitored reference glacier with a long-term in situ ELA record, using a time series of L-band SAR imagery from JERS-1, ALOS, ALOS-2, and ALOS-4. We validate the SAR-derived FLA against the in situ ELA record and find that FLA variations closely track the observed ELA changes. This agreement indicates that L-band SAR-based FLA retrieval can serve as a proxy for long-term ELA trends.

To clarify how winter observations differ between frequencies, we compare winter backscatter behavior at C-band and L-band. Winter C-band backscatter is strongly influenced by scattering from seasonal snow cover. By contrast, wintertime dry snow is largely transparent at L-band, and winter L-band SAR therefore primarily reflects surface conditions established at the end of the preceding summer. These results suggest that FLA can be monitored with a single winter L-band SAR acquisition.

How to cite: Arie, K. and Tadono, T.: Firn-Line Monitoring over the Juneau Icefield in Alaska Using SAR Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2645, https://doi.org/10.5194/egusphere-egu26-2645, 2026.

Glacier ice thickness models are fundamental to studies of glaciology, hydrology, and climatology. They play a key role in estimating ice volume, simulating future glacier evolution, and projecting meltwater runoff changes. However, ice thickness measurements (e.g., ice penetrating radar) only cover about 14% of global glacier area and disparity exists in existing ice thickness models inferred from glacier surface information, making it difficult for glaciologists to accurately simulate and project the future evolution of mountain glaciers and its impact on global sea level change and regional water supply. This study developed a 1.98 km resolution ice thickness model of the West Kunlun glaciers by inverting geophysical data surveyed through an Airbus AS350-B3e helicopter. We analyzed the errors associated with the inversion techniques, evaluated the accuracy of the ice thickness model using ice penetrating radar data, and calculated the ice volume over the surveyed region. Through model comparisons, glacier topographic features not resolvable in previously published models were identified and their potential impacts were analyzed. The ice thickness model developed in this study could provide fundamental data sets for the study of the response of glaciers to climate change and thus contributes to an improved modeling and projection of future evolution of mountain glaciers and its impact on global sea level change and regional water supply.

How to cite: Yang, J. and Shu, Q.: Ice thickness of the West Kunlun glaciers revealed by airborne geophysical survey, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4618, https://doi.org/10.5194/egusphere-egu26-4618, 2026.

EGU26-7746 | ECS | Posters on site | CR1.1

Two Decades of Glacier Mass Balance in the Southern Andes  

Mariia Usoltseva, Roland Pail, Anja Wendt, and Christoph Mayer

Glaciers are crucial components of the Earth's climate system and serve as indicators of climate change. Their substantial mass loss due to global warming significantly contributes to sea-level rise and impacts regional hydrology, downstream ecosystems and settlements. Despite considerable advancements in observational and modeling techniques, accurately quantifying glacier responses to climate change and predicting their future behavior remain complex challenges, particularly in regions characterized by rapidly changing glaciers and complex topography. In this study, we present a spatially resolved time series of annual glacier mass balance and elevation change for the Southern Andes from 2002 to 2025, derived from ASTER digital elevation models (DEMs). All available austral summer-season DEMs were compiled to minimize seasonal bias, and an automated processing workflow was developed to generate elevation change maps for the entire region as well as for individual glaciers. This approach enables consistent, large-scale monitoring without reliance on in-situ measurements, making it particularly valuable for remote and data-scarce regions. Elevation differences were converted to mass balance estimates using density assumptions, allowing both regional-scale assessments and detailed analysis of glacier complexes. Our results reveal pronounced spatial and temporal variability in glacier thinning, including periods of accelerated mass loss and localized heterogeneity linked to topographic and climatic factors. The developed methodology provides a scalable framework for long-term glacier monitoring and contributes to improved understanding of regional cryosphere dynamics and their implications for water resources and sea-level rise.

How to cite: Usoltseva, M., Pail, R., Wendt, A., and Mayer, C.: Two Decades of Glacier Mass Balance in the Southern Andes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7746, https://doi.org/10.5194/egusphere-egu26-7746, 2026.

EGU26-7945 | ECS | Orals | CR1.1

Remote sensing insights into fragmentation and decline of glaciers in the Gyama Massif of Karzok, Ladakh (1980-2025) 

Mohit Prajapati, Purushottam Kumar Garg, Sandipan Mukherjee, Supratim Guha, Ashutosh Tiwari, and Ajay Kumar Taloor

Continuous observations of glaciers are critical for measuring climate variability and understanding its consequences for regional water supplies. This study presents a comprehensive assessment of glacier changes in terms of dimension, mass balance and surface velocity in the Gyama Massif, Karzok Range, Ladakh, from 1980 to 2025. In 1980, the Gyama contained 100 glaciers characterized by a mean area of ~0.50 km² (range 0.02–4.77 km²), steep mean surface slopes of ~26° (13–41°), and high mean elevations of ~5,797 m a.s.l. (5,590–6,140 m a.s.l.), indicating predominantly small, steep, high-altitude glacier systems. The glaciers in this region experienced a total deglaciation of ~41% between 1980 and 2025. Mass-balance measurements for 100 glaciers indicate a moderately negative mean mass balance of −0.18 ± 0.10 m w.e. y-¹ for 2000–2018. Glacier flow velocities (1990–2022) exhibit a statistically significant decreasing trend of −0.13 m y-¹, corresponding to a ~75% reduction in mean velocity over the 32-year period. The average velocity of all glaciers across the study period was 4.16 m y-¹. The most pronounced areal losses occurred among the smallest glaciers: those <0.1 km² in 2000 experienced >80–100% area loss, and several glaciers disappeared completely. Glacier fragmentation increased substantially, with the number of discrete glaciers rising from 9 in 2015 to 14 in 2020 and 28 in 2025, reflecting progressive morphological disintegration associated with sustained mass loss.The substantial loss of glacier area across the Gyama Massif, together with progressive mass loss, has led to a marked slowdown in surface ice velocity, highlighting the strong coupling between glacier geometry, mass balance, and ice flow. The consistent glacier decline at very high elevations (mean ~5797 m a.s.l.) further points to the influence of elevation-dependent warming in this Trans-Himalayan region. We recommend sustained high spatio-temporal resolution remote sensing, complemented by targeted field observations, to improve glacier monitoring in this data-sparse high-altitude region. Such integrated approaches are essential for detecting glacier instability and evaluating impacts on regional hydrology and downstream water resources in the Trans-Himalaya.

Keywords: Remote sensing; Mass balance; Glacier velocity; Deglaciation; Glacier fragmentation; Ladakh Himalaya

How to cite: Prajapati, M., Garg, P. K., Mukherjee, S., Guha, S., Tiwari, A., and Taloor, A. K.: Remote sensing insights into fragmentation and decline of glaciers in the Gyama Massif of Karzok, Ladakh (1980-2025), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7945, https://doi.org/10.5194/egusphere-egu26-7945, 2026.

EGU26-8358 | ECS | Orals | CR1.1

Polythermal conditions in small glaciers in the Swiss Alps 

Janosch Beer, Mylène Jacquemart, Matthias Huss, Ilaria Santin, Gabriela Clara Racz, Christophe Ogier, Leo Hösli, Raphael Moser, James Irving, and Daniel Farinotti

Glacier thermal conditions directly influence ice mechanics, meltwater storage, and drainage, thereby governing glacier stability and hazard potential. Polythermal glaciers, in particular, can create conditions that promote ice break-offs, ice avalanches, water pocket outbursts, and even large-scale glacier detachments. Understanding their distribution is therefore critical for hazard assessment. Yet englacial temperature measurements in the Alps remain sparse and are biased toward high-elevation accumulation areas, while the thermal state of mid- and lower-elevation ablation areas is largely unknown. Extended melt seasons and refreezing of meltwater in cold firn have been associated with warming at high elevations, whereas firn loss at lower elevations may reduce meltwater retention and latent heat input. Modeling studies suggest that this imbalance can lead to cooling in ablation areas, an effect that may be particularly pronounced for very small glaciers, where internal heat production from glacier dynamics is minimal.

Here, we present a new englacial temperature dataset from six small Swiss Alpine glaciers (3000–3800 m a.s.l.), directly addressing the lack of observations in mid- to lower-elevation ablation areas that are poorly constrained by existing measurements. The dataset combines borehole thermometry with ground-penetrating radar surveys. Polythermal conditions were identified in three glaciers, with the cold–temperate transition surface (CTS) occurring at depths of 14–25 m. Below the seasonal surface layer, ice temperatures generally ranged from temperate conditions to –2.1 °C. Two of the glaciers exhibit a recurring pattern in which temperate ice at higher elevations transitions downslope into fully or partially frozen glacier tongues. At the third polythermal site, the CTS was detected at several locations between 17 and 22 m depth, while basal thermal conditions remain partly unresolved. One glacier appears predominantly cold, and at two additional sites, shallow thermistors recorded year-round cold conditions within the seasonal layer, while temperate ice at depth cannot be ruled out. Ground-penetrating radar reflectivity is generally consistent with borehole-derived thermal conditions, characterized by low reflectivity in cold ice and enhanced reflectivity in temperate zones. Our findings suggest that polythermal-type glaciers in the European Alps may be more widespread than previously recognized, with important implications for glacial hazard assessment and for understanding climate-driven changes in smaller Alpine glaciers.

How to cite: Beer, J., Jacquemart, M., Huss, M., Santin, I., Clara Racz, G., Ogier, C., Hösli, L., Moser, R., Irving, J., and Farinotti, D.: Polythermal conditions in small glaciers in the Swiss Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8358, https://doi.org/10.5194/egusphere-egu26-8358, 2026.

EGU26-9325 | ECS | Posters on site | CR1.1

Glacier elevation change estimates: decoding the systematic differences between radar altimetry and DEM differencing 

Anne Guyez, Etienne Berthier, Livia Jakob, Noel Gourmelen, Livia Piermattei, Clare Webster, Samuel U. Nussbaumer, Michael Zemp, Joaquín M.C. Belart, and Tómas Jóhannesson

Measuring glacier mass change worldwide is essential to document the impact of climate change, understand glacier-related hazards and assess the contribution of the cryosphere to sea-level rise. Over the last two decades, three remote-sensing techniques have been used to measure glacier mass change: digital elevation model (DEM) differencing, altimetry and gravimetry. The Glacier Mass Balance Intercomparison Exercise (GlaMBIE, ESA-funded) aims to compile, homogenize and combine these regional glacier mass change observations.  

 

One intriguing outcome from the first GlaMBIE phase (2022–24) was a systematic difference of region-wide elevation change measured using ASTER DEM differencing (dDEM) and CryoSat-2 radar altimetry. In most cases, dDEM resulted in more negative values in all glacier regions with an average regional difference of 0.08 ± 0.07 m w.e. yr-1 (The GlaMBIE Team, 2025). The work presented here is part of the second GlaMBIE phase (2025–27). It aims at describing in more detail and understanding the differences between these two techniques. We focus on major Icelandic ice caps as test sites as they present a good coverage for both techniques and are also covered with high resolution, precise dDEM data (e.g., airborne lidar in 2013 and Pléiades in 2020 for Hofsjökull ice cap).  

 

Our preliminary results indicate that the differences between published ASTER (Hugonnet et al., 2021) and CryoSat-2 (Jakob and Gourmelen, 2023) estimates are also found at ice cap and glacier scale. Next, we plan to compare the methods over the exact same period, and evaluate them using accurate validation data. We will also test the sensitivity to the software used to generate the DEMs, to alternative processing of CryoSat-2 data, and to the post-processing of the data (altimetry and DEMs) to find the key reasons for the systematic difference.

How to cite: Guyez, A., Berthier, E., Jakob, L., Gourmelen, N., Piermattei, L., Webster, C., U. Nussbaumer, S., Zemp, M., M.C. Belart, J., and Jóhannesson, T.: Glacier elevation change estimates: decoding the systematic differences between radar altimetry and DEM differencing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9325, https://doi.org/10.5194/egusphere-egu26-9325, 2026.

EGU26-9409 | Orals | CR1.1

4D Multi-View Stereo Reconstruction for High-Resolution Calving Monitoring of Glacier Perito Moreno: A Basis for Dynamic Analysis and Prediction 

Laura Camila Duran Vergara, Bindusara Nagathihalli Lokesh, Xabier Blanch Gorriz, and Anette Eltner

In this study, we present a high temporal resolution (30-minute) multi-view stereo (MVS) photogrammetric dataset capturing the front of the lake-terminating Perito Moreno Glacier during daylight over more than one year. We aim to provide novel data to investigate glacier dynamics, which are strongly affected by climate change and pose increasing risks to ecosystems and human infrastructure. The images for the photogrammetric reconstruction are automatically inspected and prepared to create high-precision 4D (3D + time) point clouds, which are then compared per epoch to detect surface changes along an approx. 300 m wide study reach.

The MVS system comprises eight DSLR cameras and uses 4G connectivity for daily data transfer, aiming for near-real-time monitoring. This has resulted in more than 75,000 images stored on a central server, which allows the calving analysis based on more than 5,000 models. To isolate image regions relevant for the generation of dense clouds with maximum precision across as many epochs as possible, the images are segmented using the artificial intelligence (AI)-based image segmentation model SAM2. The relevant regions are assessed using blur metrics, which identify low contrast caused by harsh glacier conditions, such as moisture or water droplets, thereby reducing the risk of including images of low quality that interfere with image correlation success.

The results of our image pre-processing demonstrate that lighting conditions have the greatest impact on image segmentation performance. In contrast, the final model quality of the 4D point cloud reconstructions, which are based on a multi-epoch multi-imagery (MEMI) strategy, is mostly affected by the presence of adjacent dynamically changing regions, such as floating ice on the lake, highlighting the need for masking these regions. Applying masking further seems to improve the robustness of detecting subtle glacier surface changes, which is essential for pre-failure deformation analysis, providing valuable input for future calving prediction efforts.

The point cloud sequences are analyzed using the Multiscale Model to Model Cloud Comparison (M3C2) algorithm to quantify surface changes. Although calibration parameters of focal length and principal point exhibit temporal variability, a constant calibration strategy is examined to ensure consistent alignment across all epochs, which furthermore enables the observation of glacier flow velocities in both horizontal and vertical directions. Initial results for a test period during a week in summer indicate that a constant calibration does not adversely affect model generation, suggesting that calibration stability may be sufficient under favorable summer conditions, while ongoing analyses will assess the robustness during winter months. Current efforts focus on refining dense cloud quality by separating glacier surfaces from points reconstructed on stable rock areas, which were intentionally retained during point cloud generation to provide stable reference regions for the MEMI workflow.

Our introduced workflow enables the creation of a reliable calving inventory, exceeding the spatio-temporal resolution of conventional glacier monitoring techniques. In a next step, we aim to combine the created calving inventory with associated dynamic parameters, such as glacier velocity, and with environmental variables to support the development of AI-based calving prediction models.

How to cite: Duran Vergara, L. C., Nagathihalli Lokesh, B., Blanch Gorriz, X., and Eltner, A.: 4D Multi-View Stereo Reconstruction for High-Resolution Calving Monitoring of Glacier Perito Moreno: A Basis for Dynamic Analysis and Prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9409, https://doi.org/10.5194/egusphere-egu26-9409, 2026.

EGU26-9511 | Orals | CR1.1

Monitoring of Antarctic Peninsula glacier terminus area change and ice surface velocity using dense satellite time series 

Sarah Leibrock, Ross A. W. Slater, Anna E. Hogg, and Celia A. Baumhoer

The Antarctic Peninsula is among the most rapidly warming regions on Earth and has experienced widespread glacier retreat and acceleration since at least the 1980s, with significant implications for global sea level rise. Glacier change in this region unfolds across a wide range of timescales, spanning from short-lived dynamic events that can trigger persistent adjustments to recurring seasonal variability. However, Earth observation datasets that capture glaciological variables such as ice velocity or calving front dynamics at intra-annual timescales remain scarce. This is largely due to the small size and fast ice flow of Antarctic Peninsula glaciers, combined with complex topography, variable climate, and extreme weather conditions.

Here, we address this observational gap by leveraging a newly developed dataset of sub-seasonal terminus area change records (2013–2023) together with high-resolution satellite-derived ice surface velocity measurements (2014– 2024) to investigate the dynamics of 42 key outlet glaciers on the northern Antarctic Peninsula.

Our results reveal widespread glacier retreat and acceleration, with cumulative ice loss amounting to ~279 km². The majority of this loss (73 %) was observed for glaciers on the eastern Antarctic Peninsula, particularly within the Larsen B embayment, and is attributed to major calving events in early 2022. Although 71 % of the glaciers accelerated over the study period, most eastern glaciers displayed slight trends of slowdown – except for those in the Larsen B embayment, where initial deceleration was followed by abrupt and pronounced velocity increases after the calving events, with some glaciers more than doubling their flow speed. Seasonal analysis further indicates substantial inter-annual variability, with two-thirds of glaciers exhibiting strong seasonal velocity fluctuations, and around half displaying comparable signals in terminus area change.

Overall, the findings demonstrate the persistence of long-term trends of glacier retreat and flow acceleration, while also highlighting substantial spatial and temporal heterogeneity in glacier dynamics across the region, underscoring the need for temporally and spatially detailed monitoring.

How to cite: Leibrock, S., Slater, R. A. W., Hogg, A. E., and Baumhoer, C. A.: Monitoring of Antarctic Peninsula glacier terminus area change and ice surface velocity using dense satellite time series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9511, https://doi.org/10.5194/egusphere-egu26-9511, 2026.

EGU26-10689 | ECS | Posters on site | CR1.1

Elevation Change of Icelandic Glaciers from TanDEM‑X DEM Differencing with Penetration‑Bias‑Optimized Scene Selection  

Lukas Krieger, Codruț-Andrei Diaconu, Sahra Abdullahi, Sindhu Ramanath, and Dana Floricioiu

Mapping of elevation changes across large glacier regions is an essential basis for future IPCC reports. The first Glacier Mass Balance Intercomparison Exercise (GlaMBIE) established a community estimate of global glacier mass change [1]. However, the method of InSAR DEM differencing remains an underrepresented data source in this experiment.

For the second GlaMBIE data contribution, we aim to update our existing DEM Differencing processing pipeline [2]. It will be implemented on the high performance “Terrabyte” platform at the Earth Observation Center (EOC) of DLR. Unlike our previous contribution [2], which relied on targeted acquisitions to cover entire glacier regions, we will exploit the existing TanDEM‑X catalogue. This strategy facilitates future processing of large glacierized regions worldwide.

Recent advances regarding the uncertainty assessment of TanDEM-X DEM Differences will be fully incorporated in this pipeline [3, 4]. Special attention is given to reducing possible biases due to signal penetration. This bias is mitigated by differencing carefully selected TanDEM-X acquisitions from the same season with unchanged SAR geometry, reducing penetration differences between DEMs. Moreover, the relative importance of SAR signal penetration for accurate mass balance measurements also reduces with the length of the observation period.

In this work we will calculate the elevation change of all glacierized regions in Iceland based on available acquisitions in the TanDEM-X catalogue. Because the majority of TanDEM-X data were originally tasked and intended for the TanDEM-X Global DEMs, the final coverage will naturally gravitate towards these acquisitions, however alternative more suitable scenes in the catalogue will be substituted. A penetration-bias-optimized coverage for Iceland is best achieved by targeting the 2013 - 2021 period, with replacement scenes from other times possible.

We will investigate several spatial and temporal extrapolation strategies to fill gaps in Icelandic glacier coverage that must be left intentionally without measurements because the only available scenes are suspected of being affected by signal‑penetration biases.

References

[1]        Zemp, M., Jakob, L., Dussaillant, I., Nussbaumer, S. U., Gourmelen, N., Dubber, S., A, G., Abdullahi, S., Andreassen, L. M., Berthier, E., Bhattacharya, A., Blazquez, A., Boehm Vock, L. F., Bolch, T., Box, J., Braun, M. H., Brun, F., Cicero, E., Colgan, W., … The GlaMBIE Team. (2025). Community estimate of global glacier mass changes from 2000 to 2023. Nature, 1–7. https://doi.org/10.1038/s41586-024-08545-z

[2]        Abdel Jaber, W., Rott, H., Floricioiu, D., Wuite, J., & Miranda, N. (2019). Heterogeneous spatial and temporal pattern of surface elevation change and mass balance of the Patagonian ice fields between 2000 and 2016. The Cryosphere, 13(9), 2511–2535. https://doi.org/10.5194/tc-13-2511-2019

[3]        Hugonnet, R., Brun, F., Berthier, E., Dehecq, A., Mannerfelt, E. S., Eckert, N., & Farinotti, D. (2022). Uncertainty Analysis of Digital Elevation Models by Spatial Inference From Stable Terrain. IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, 15, 6456–6472. IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing. https://doi.org/10.1109/JSTARS.2022.3188922

[4]        Li, S., & Hajnsek, I. (2025). Geodetic glacier mass balance in the Karakoram (2011–2019) from TanDEM-X: An InSAR DEM differencing framework. Remote Sensing of Environment, 331, 115023. https://doi.org/10.1016/j.rse.2025.115023

How to cite: Krieger, L., Diaconu, C.-A., Abdullahi, S., Ramanath, S., and Floricioiu, D.: Elevation Change of Icelandic Glaciers from TanDEM‑X DEM Differencing with Penetration‑Bias‑Optimized Scene Selection , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10689, https://doi.org/10.5194/egusphere-egu26-10689, 2026.

EGU26-11729 | Orals | CR1.1

Comparing approaches for glacier elevation change estimation using optical DEM time series 

Clare Webster, Francesco Ioli, Joaquín M.C. Belart, Tómas Jóhannesson, Etienne Berthier, Enrico Mattea, Robert McNabb, Désirée Treichler, Luc Girod, Michael Zemp, and Livia Piermattei

Digital elevation models (DEMs) from optical stereo satellite imagery are widely used to quantify glacier elevation change through DEM differencing. However, incomplete spatial coverage and irregular temporal sampling limit the applicability of standard pair-wise DEM differencing over large glaciers, requiring the analysis of multi-temporal DEM time series.

Here, we compare methodological approaches for interpolating optical DEM time series to derive mean glacier elevation change rates using freely available datasets. We exploit SPOT-5 and ArcticDEM as high-resolution complements to the ASTER DEM record. Using the Hofsjökull ice cap (Iceland) as a pilot study, we assess the performance and transferability of a pixel-based Gaussian interpolation approach (Hugonnet et al., 2021) and introduce a computationally efficient elevation-band-based method. Validation is performed against independent elevation datasets, such as LiDAR and Pléiades, and through pairwise DEM differencing. 

Our results show that the elevation-band approach provides reliable estimates of glacier-elevation change under sparse, irregular sampling conditions. Furthermore, with its low computational cost and flexibility, the method is well-suited for regional applications and for extending geodetic glacier mass-balance assessments beyond the ASTER era.

 

Hugonnet, R., McNabb, R., Berthier, E., Menounos, B., Nuth, C., Girod, L., Farinotti, D., Huss, M., Dussaillant, I., Brun, F. and Kääb, A., 2021. Accelerated global glacier mass loss in the early twenty-first century. Nature, 592(7856), pp.726-731.

How to cite: Webster, C., Ioli, F., Belart, J. M. C., Jóhannesson, T., Berthier, E., Mattea, E., McNabb, R., Treichler, D., Girod, L., Zemp, M., and Piermattei, L.: Comparing approaches for glacier elevation change estimation using optical DEM time series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11729, https://doi.org/10.5194/egusphere-egu26-11729, 2026.

Mass balance models are typically evaluated using a sparse collection of point measurements on one or more glaciers. Discrete measurements of mass or elevation loss often reflect surface elevation/mass change along centreline ablation stakes. More recent approaches use geodetic data to help constrain these mass balance models, but the infrequent nature of these distributed datasets often precludes an evaluation of how well these models capture important physical properties such as albedo evolution, short-term events such as impurity deposition following wildfire or dust loading, or the importance of heat waves. Here we describe the unique observational dataset for Place Glacier, a small (2 km2) benchmark glacier monitored since 1965. Our dataset includes 62 airborne laser altimetic and 30 hyperspectral surveys from which we derive monthly surface elevation change and optical retrievals (e.g. grain size, albedo and radiative forcing caused by light-absorbing particles-LAPs) during the ablation seasons (2020-2025). These 2-m data are currently being used to assess the performance of distributed surface mass balance models such as COSIPY, GEMB, CROCUS. The dense observational record allows us to perform suitable calibration and validation exercises for each model but also for spaceborne-derived datasets of surface elevation and albedo change. Surface mass balance model performance during the validation period is typically excellent, but significantly degrades when attempting to simulate mass change prior to 2020. Factors which account for this poor pre-2020 performance includes major changes in the extent of firn, late-lying snow and impurity deposition. In addition to elevated flux of LAPs from dry and wet deposition, thinning of firn has elevated surface concentration of LAPs and surface debris thereby darkening the glacier and accelerating mass loss. Work is underway to physically model these important physical processes leading to albedo reduction and attendant glacier mass loss.  

How to cite: Menounos, B. and Viner, N.: Surface elevation change and optical retrieval products to benchmark the next generation of surface mass balance models, Place Glacier, Canada, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11825, https://doi.org/10.5194/egusphere-egu26-11825, 2026.

EGU26-12452 | Orals | CR1.1

Glacier surging in the Karakoram continues unabated 

Frank Paul

The Karakoram mountain range is well-known for its numerous surge-type glaciers of which several have recently surged or are currently surging. Analysis of historic satellite images, topographic maps and reports revealed repeat surges for many of the glaciers, partly back to the 19th century. The observed surges display a great variety of characteristics regarding surge durations, repeat cycles, flow velocities, advance rates and mass transfer patterns. However, surge mechanisms remain speculative, as the thermal and basal conditions of the glaciers are largely unknown.

Along with positive glacier mass balances and decreasing summer temperatures, the enhanced surge activity in this region is one part of the so-called Karakoram Anomaly. It has been speculated that the Karakoram Anomaly might come to an end, as its mass balance part is showing increasingly negative values, i.e. more similar to the glaciers in surrounding mountain ranges. However, dense time-series of freely available satellite images reveal that this is so far not reflected in a diminishing surge activity, which instead continues unabated.

For this study, animations of Sentinel-2 image quicklooks have been used for early detection of upcoming surges and an analysis of surge development over the past ten years in the central Karakoram. While tributary glaciers continued surging according to their surge cycles, also the much larger trunk glaciers (Panmah and Sarpo Laggo) are now surging again and deform or erase the surge marks of previous tributary surges. In 2024/25, at least 15 glaciers were surging in a small region of the Karakoram, two of which were not classified as of surge-type before. Apart from the animations revealing surge front migration and glacier interactions, time series of flow velocities and surface elevations reveal strong differences in surge dynamics among the glaciers. The 10 m resolution of Sentinel-2 is at the edge of providing meaningful velocity data for the 7 smallest glaciers in the sample.

How to cite: Paul, F.: Glacier surging in the Karakoram continues unabated, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12452, https://doi.org/10.5194/egusphere-egu26-12452, 2026.

EGU26-13647 | ECS | Posters on site | CR1.1

Exploring contemporaneous observational datasets to derive glacier surface mass balance from continuity approaches (ContinuIX working group) 

Maaike Izeboud, Albin Wells, Johannes J. Fürst, Marin Kneib, Evan Miles, Victor Devaux-Chupin, Lander Van Tricht, Katarina Henning, and Harry Zekollari

The surface mass balance (SMB) of glaciers represents a direct link to the local climate and is a key variable in modelling glacier response to climate change. While the SMB is traditionally measured at point locations with ablation stakes or snowpits, recent advances allow estimation of spatially distributed SMB using remotely sensed data of surface elevation change, ice velocity, and ice thickness by solving the mass continuity equation. Such inverse approaches offer a promising alternative to field-based SMB data collection, particularly for model calibration and large-scale assessments. However, SMB inversion approaches vary in spatial coverage, assumptions, and solution strategies as well as in using data of different resolutions and temporal consistency—raising questions about their comparability, performance, and uncertainties.

The Continuity approaches for mass balance Intercomparison eXercise (ContinuIX) is a community effort organized through an IACS Working Group that aims to compare existing continuity approaches for SMB estimation and to deliver clear guidelines and recommendations for future developers and users of SMB products derived from these methods. The first objective of ContinuIX focuses on compiling a benchmark dataset with high-quality, contemporaneous observational data (surface elevation change, velocity, thickness, and in situ SMB), as well as controlled synthetic test cases. The next activities will involve a structured intercomparison experiment using these best possible datasets to assess differences between approaches.

Here, we present progress on the benchmark dataset of phase one, which includes extensive contemporaneous observations of eight glaciers across multiple regions. This dataset may be of value for a wide range of glaciological studies. Additionally, we apply and present first results of mass continuity methods to demonstrate how distributed SMB products can be derived, providing a preview of the types of comparisons envisioned for the next objective of ContinuIX. This presentation is intended not only to share initial results, but also to invite input and discussion from the community as we shape the next steps of ContinuIX. We particularly welcome ideas, feedback, and expressions of interest from potential contributors or users of continuity-derived SMB products.

How to cite: Izeboud, M., Wells, A., Fürst, J. J., Kneib, M., Miles, E., Devaux-Chupin, V., Van Tricht, L., Henning, K., and Zekollari, H.: Exploring contemporaneous observational datasets to derive glacier surface mass balance from continuity approaches (ContinuIX working group), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13647, https://doi.org/10.5194/egusphere-egu26-13647, 2026.

EGU26-14880 | Posters on site | CR1.1

Remote sensing of North Greenland glaciers from the 1970s to present 

Robert McNabb

The Arctic is one of the fastest-warming regions in a rapidly warming world. Arctic glaciers are an important contributor to sea level rise, and their increased mass change and retreat has impacts ranging from local-scale ecosystems to regional-scale changes in ocean chemistry and circulation. Longer-term observations, especially of elevation and volume changes, are key for understanding and constraining predictions of future sea level change and other environmental impacts.

Over recent decades, peripheral glaciers in Greenland north of 79° latitude showed fairly steady rates of negative mass balance and small rates of area change, in spite of strongly increased regional warming. In this study, we combine a broad range of remotely sensed imagery and datasets to observe decade-scale changes to peripheral glaciers in the North of Greenland over a 50 year time period. We use historical aerial and declassified satellite imagery as well as Landsat and Sentinel-2 scenes to map glacier area across each decade through a semi-automated approach. To map accumulation area ratio (AAR) for each time period, we apply an albedo threshold approach that has been used to differentiate between snow and bare ice in other regions. Finally, we derive elevation changes using a combinaton of historic aerial and satellite-derived digital elevation models (DEMs) from the 1970s, the ArcticDEM, and ASTER and SPOT-5 derived DEMs to observe elevation and volume changes over the same time period. With the benefit of multiple glacier inventories, we also evaluate the impact of deriving geodetic mass balances from glacier outlines at different points in time.

How to cite: McNabb, R.: Remote sensing of North Greenland glaciers from the 1970s to present, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14880, https://doi.org/10.5194/egusphere-egu26-14880, 2026.

EGU26-17071 | ECS | Posters on site | CR1.1

Observation of mass balance and flow of very small glaciers in northern Japanese Alps. 

Yukako Takehana, Chiyuki Narama, and Kenshiro Arie

Nine very small glaciers (VSGs) have been identified in the northern Japanese Alps (e.g., Fukui et al., 2018; Arie et al., 2025). These VSGs persist under relatively warm conditions at elevations around 2,000 m, where the mean annual air temperature is approximately 2–3  ℃. Understanding the mechanism that enables their persistence is therefore an important scientific issue. However, long-term mass-balance observations and understanding of the flow mechanisms remain limited.

In this study, the mass balance of eight glaciers and perennial snow patch was observed from the 1960s to 2025, and interannual and seasonal variations in flow velocity were investigated at the Shakushizawa Glacier. The studied glaciers and snow patches―Hakubazawa, Shakushizawa, Kaerazuzawa, Karamatsuzawa, Kakunezato, Komado, Sannomado, Gozenzawa―are located at elevations of 1,700-2,700 m and are characterized by heavy snow accumulation (snow depth: 20-30 m) due to the northwesterly winter monsoon and frequent avalanches.

Cumulative mass balance from the 1960s to the mid-2010s showed only slight gains or losses; however, following the low-snowfall year of 2016, all glaciers and perennial snow patches experienced substantial mass loss by 2025. Meteorological observations (Hakuba AMeDAS) and ERA5 reanalysis data indicate no significant long-term decrease in snowfall since the 1950s, whereas melt amounts estimated using both an energy-balanzsce and a degree-day methods show an increasing trend. These results suggest that the recent acceleration of mass loss is mainly driven by enhanced summer melting associated with rising air temperatures.

Flow observations at the Shakushizawa Glacier show that annual flow velocities exceed those observed at the end of melt season, implying either accelerated internal deformation under heavy winter snow load or enhanced basal sliding during the early melt season. 

How to cite: Takehana, Y., Narama, C., and Arie, K.: Observation of mass balance and flow of very small glaciers in northern Japanese Alps., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17071, https://doi.org/10.5194/egusphere-egu26-17071, 2026.

EGU26-17333 | ECS | Orals | CR1.1

Long-term variations of glacier albedo from 1993 to 2025 in the Central Hunza basin 

Blanka Barbagallo, Davide Fugazza, and Guglielmina Adele Diolaiuti

Glacier surface albedo is an important factor affecting glacier ablation, and it plays a crucial role in understanding glacier health and the surface energy balance. However, its temporal and spatial distribution on glaciers is frequently ignored, entailing the use of constant values in melt models, which can cause inaccurate melt estimates. Glacier albedo changes in the 21st century remain poorly understood.

Past studies highlight a decrease in glacier albedo between 2001 and 2021 in most regions of the Third Pole. However, the glacier response to climate change in the Karakoram region is not fully understood. A large portion of the glacierized area has shown unusual behavior with respect to global glacier shrinkage, commonly known as the “Karakoram Anomaly”.

In this study, we analyzed, both temporally and spatially, the long-term trend of summer glacier albedo from 1993 to 2025, using Landsat 4/5 TM, 7 EMT+, and 8/9 OLI data from Google Earth Engine database. Our study focuses on the Central Hunza basin, a large basin (2383 km2) in Karakoram (Pakistan), hosting around 280 glaciers. This basin has already shown, on average, an almost balanced mass budget in the period 1973-2009. To ensure focusing only on snow free glacier surface albedo, we masked out snow covered areas by means of the OTSU algorithm and also assessed the Snow Line Altitude, in order to investigate also its variations at the glacier and basin scale. To assure data continuity across sensors with different spectral resolution, we performed a harmonization of the Landsat data.

This study emphasizes the importance of not assuming albedo as a constant, since its long-term variability in the region may not follow global trends. This is particularly relevant as glaciers act as the main hydrological resource in this region.

How to cite: Barbagallo, B., Fugazza, D., and Diolaiuti, G. A.: Long-term variations of glacier albedo from 1993 to 2025 in the Central Hunza basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17333, https://doi.org/10.5194/egusphere-egu26-17333, 2026.

EGU26-17768 | ECS | Orals | CR1.1

Glacier mass changes in the Western Pamirs during 2003-2025 from high-resolution stereo satellite images 

Haruki Hagiwara, Evan Miles, Achille Jouberton, Jose Muñoz Hermosilla, Shaoting Ren, Thomas E. Shaw, Joel Fiddes, Amaury Dehecq, Romain Hugonnet, and Francesca Pellicciotti

The Pamir Mountains are a key focus of research on the response of glaciers to climate change in High Mountain Asia. They constitute an important mountain water tower that is highly vulnerable to future climatic and environmental change, and they host glaciers that experienced limited but increasing mass loss during 2000-2019. Few studies have constrained mass balance in detail within the region, and these have highlighted strong spatio-temporal variability. Quantification of glacier mass changes and their drivers is challenged by sparse in situ data, strong East-West gradients of temperature and precipitation, and complex glacier processes including debris cover, surging behavior, and collapse features. In this study, we focus on 41 glaciers in the Sangvor region of the western Pamir for 2003-2025 to: i) evaluate the robustness of previous estimates of mass losses for 2000-2019, ii) identify glacier trajectories beyond 2019, and iii) understand the influence of surging glaciers on the observed mass changes. We adopted a stereo image-processing workflow from the Ames Stereo Pipeline and generated DEMs from SPOT5, SPOT6, and Pléiades stereo satellite imagery. Glacier mass balance for each time series was derived using current best practices for DEM co-registration, bias correction, and uncertainty propagation. Additionally, we applied new algorithms for jitter correction, seasonal snow correction based on in-situ data, and a duration-dependent correction scheme for volume-to-mass conversion uncertainties.

 

Our results provide a time series of high-resolution geodetic surface height changes and glacier mass balance over seven sub-periods spanning 2003 to 2025: -0.19 ± 0.04 m w.e. a-1 for 2003-2019, -0.63 ± 0.05 m w.e. a-1 for 2019-2025, and -0.28 ± 0.02 m w.e. a-1 for the entire period of 2003-2025 for three key intervals. Our 2003-2019 results agree with the mean mass balance measured by ASTER for 2000-2019 (-0.21 m w.e. a-1) and with the temporal trend. We highlight a sharp mass gain (0.16 ± 0.03 m w.e. a-1) between 2014 and 2019, followed by a pronounced progressive shift toward negative mass balances. During 2019-2025, characterized by exceptionally warm and dry conditions, the mass balance has been increasingly negative despite higher uncertainty in our annual estimates, reaching its maximum loss of -1.45 (+0.51/-0.19) m w.e. a-1 in 2024-2025. We also find no statistically significant difference between the mass balance of surging glaciers and the regional mean for the periods of our study. Overall, our results reveal strong temporal variability in glacier mass balance in the region. While long-term mean mass balances agree with previous ASTER-based estimates, our high-resolution geodetic time series resolves their short-term variability, illuminating a complex evolution that includes a marked mass gain for 2014-2019 and a rapid shift toward strongly negative balances thereafter. Comparison with reanalysis data suggests that this variability is more closely linked to precipitation anomalies than to temperature, suggesting a dominant role of mass accumulation and snowfall variability. These results demonstrate the value of high-resolution stereo imagery and motivate extension to the wider Pamir region and can form a new, high-resolution baseline for modelling projections of future glacier changes in the region.

How to cite: Hagiwara, H., Miles, E., Jouberton, A., Muñoz Hermosilla, J., Ren, S., E. Shaw, T., Fiddes, J., Dehecq, A., Hugonnet, R., and Pellicciotti, F.: Glacier mass changes in the Western Pamirs during 2003-2025 from high-resolution stereo satellite images, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17768, https://doi.org/10.5194/egusphere-egu26-17768, 2026.

EGU26-18052 | ECS | Orals | CR1.1

Mapping bedrock topography and ice thickness distribution of Patagonian outlet glaciers using ground-penetrating radar 

Moritz Koch, Christian Sommer, Norbert Blindow, Jorge Berkhoff, Pedro Skvarca, Johannes Fürst, and Matthias Holger Braun

The Southern Patagonian Icefield, the largest temperate ice body in the Southern Hemisphere, is among the regions with the highest mass-loss rates globally. Most of this mass loss is driven by large, water-terminating outlet glaciers. Their response to climate change, however, is heterogeneous in time and space. For water-terminating glaciers, subglacial topography plays a key role in modulating their response to climate change, yet it remains largely unknown, especially near glacier termini.

We present results from two campaigns in 2022 and 2024, during which we conducted helicopter-borne GPR measurements of three of the largest Argentine outlet glaciers: Glaciar Upsala, Glaciar Viedma, and Glaciar Perito Moreno. Our measurements, covering 232 km of flight tracks, reveal the complex subglacial topography in the lower regions of these glaciers and show bed reflections of up to 800 m depth at Glaciar Upsala. Our data also shows Glaciar Perito Moreno lies on a pronounced subglacial bedrock ridge, which has largely contributed to its past stability.

In addition, we incorporated our measurements into an established ice-thickness reconstruction to derive the basin-wide ice-thickness distribution and, thus, the subglacial topography. Our ice-thickness maps indicate that the three glaciers had a combined ice volume of 831 km³ in the year 2000, which is more than six times the total ice volume of the European Alps combined.

While the rerteat of Glaciar Upsala and Viedma has slowed down, Glaciar Perito Moreno shows increased surface-lowering rates, from 0.34 m a⁻¹ (2000-2019) to 5.5 m a⁻¹ (2019-2024), accompanied by glacier acceleration and frontal retreat. After almost 100 years, the glacier has started to detach from its pinning point. Using a simple numerical model, we show that buoyancy-driven retreat of several kilometres could occur in the near future if lowering rates persist.

 

How to cite: Koch, M., Sommer, C., Blindow, N., Berkhoff, J., Skvarca, P., Fürst, J., and Braun, M. H.: Mapping bedrock topography and ice thickness distribution of Patagonian outlet glaciers using ground-penetrating radar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18052, https://doi.org/10.5194/egusphere-egu26-18052, 2026.

EGU26-18630 | Orals | CR1.1

Passive acoustic signatures of frontal ablation at tidewater glaciers in the Antarctic Peninsula and Greenland 

Hari Vishnu, Mandar Chitre, and Matthias Hoffmann-Kuhnt

Tidewater glaciers in the Arctic and the Antarctic Peninsula are undergoing an unprecedented level of retreat owing to rising temperatures, driven by both ocean-induced melting and atmospheric warming of ice-sheets. Frontal ablation at tidewater glaciers occurs primarily through calving and submarine melting, each of which generates distinct sounds that can be detected using acoustic sensing. Calving generates impulsive transient sounds associated with the impact of the ice on the ocean surface, whereas submarine melting generates a more persistent acoustic signal due to release of pressurized bubbles trapped within the ice. These characteristics provide the opportunity to remotely monitor glacier frontal ablation over a long term using passive acoustics, and complement other modalities of glacial remote sensing. To better understand the physical acoustic variability in glacial bays, we undertook acoustic recordings in tidewater glacier bays in Greenland and the Antarctic Peninsula in 2024-2025 using a long vertical hydrophone array, which allows discrimination of sound emanating from glacier terminus melt. These measurements reveal the directionality of the melt-induced sound field, wide variation in acoustic levels and spatial, temporal and spectral characteristics in the acoustic field in the different glacial bays, and significant contributions from melting ice mélange. These were coupled with conductivity-temperature-depth measurements to understand the effect of thermohaline structure on the melt-induced acoustic field. We investigate the acoustic field characteristics including the directionality, spectrum and coherence, potential links with the water temperature in the bay, and place our findings in the context of earlier passive acoustic studies conducted in Svalbard during 2019-2023, drawing comparisons and contrasts across polar regions. Together, these advance the use of passive acoustics as a tool for long-term, remote monitoring of tidewater glacier ablation.

How to cite: Vishnu, H., Chitre, M., and Hoffmann-Kuhnt, M.: Passive acoustic signatures of frontal ablation at tidewater glaciers in the Antarctic Peninsula and Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18630, https://doi.org/10.5194/egusphere-egu26-18630, 2026.

EGU26-19130 | ECS | Orals | CR1.1

 Accelerated ice-mass loss in southern Patagonia observed by satellite gravimetry 

Abelardo Romero, Andreas Richter, Thorben Döhne, Martin Horwath, Eric Mardewald, and Federico Suad Corbetta

Southern Patagonia hosts the largest accumulation of ice in South America. The Patagonian Icefields (PI), situated just north of 52° S, with a highly fragmented glacier outline and a N-S orientation represent the largest glacial system in the region with surface areas of 4,000 and 12,000 km², respectively. A smaller ice cap covers the Cordillera Darwin (CD, 2600 km²) in the south-western part of the Tierra del Fuego main island. The Gran Campo Nevado (GCN, 200 km²) is situated halfway between the Southern Patagonian Icefield and CD. The area of the PI is subject to intense glacial isostatic adjustment (GIA) effects due to its particular rheological setting as response to relatively recent ice-mass loss. These effects include observed bedrock uplift and gravity field changes. Continuous monitoring of the ice loss in Patagonia is key to understanding the impact of ongoing climate change in the southern mid-latitudes and the southeastern Pacific. Previously published mass-balance estimates for the PI agree in an intense ice-mass loss, but indicate a dependence on the analyzed period and the applied method. The GRACE (2002-2017) and GRACE-Follow On (GRACE-FO, since 2018) missions provide an efficient tool for quantifying mass redistribution on Earth from satellite gravimetry data. Richter et al. (2019) developed a method to determine a mass change time series of the PI over the 15-years period of the GRACE mission. By applying a series of corrections, the gravimetric effects of simultaneous mass redistribution processes are removed from the pseudo-observables in order to isolate the target mass-change signal prior to the inversion. We present a new ice-mass change time series extending our estimation of the PI over CD and GCN, and including the GRACE-FO data record over a time span of 22 years. It benefits from improved models used to correct for the gravity effects of GIA, ocean mass redistribution, continental water storage variations, and ice-mass changes of the polar ice sheets and mountain glaciers outside Patagonia. In addition, the effects of major earthquakes in the study region are corrected, and recent InSAR remote-sensing results are incorporated as a priori information on the spatial distribution of ice-mass changes in Southern Patagonia. Our results confirm a steady ice-mass loss with a mean rate of -30 Gt/a and reveal an increase in the mass-loss rate during most recent years, reaching values of about −43 Gt/a.

How to cite: Romero, A., Richter, A., Döhne, T., Horwath, M., Mardewald, E., and Suad Corbetta, F.:  Accelerated ice-mass loss in southern Patagonia observed by satellite gravimetry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19130, https://doi.org/10.5194/egusphere-egu26-19130, 2026.

EGU26-19873 | ECS | Posters on site | CR1.1

Calculating Snowline Altitudes on Glaciers with Patchy and Irregular Snow Cover Using Satellite Imagery 

Mhairi Hallford, Brice R. Rea, Matteo Spagnolo, Lydia Sam, Shaktiman Singh, and Donal Mullan

Previous studies have mapped end-of-season snowlines (ESS) on glaciers from satellite imagery to find their snowline altitudes (SLA) to use as a proxy for the glacier equilibrium line altitude (ELA). A line is traced along the boundary between snow and ice, then, from a digital elevation model (DEM), elevation values are extracted at regular intervals along the line. The average elevation of these points is taken to be the SLA. While this approach would be advantageous, as it offers a solution to measuring glacier ELAs in remote regions, it is prone to an oversampling bias. Where snow cover is patchy, for example, in shaded areas or where avalanching has occurred, a greater length of line is mapped in order to follow the snow-ice boundary than is required for smoother segments. This is regardless of whether the region contributes a larger area of snow cover or not. Consequently, SLA calculations are prone to oversampling from areas of irregular snow cover. Even when the ESS is mapped accurately and precisely, the SLA value may differ significantly from the true ELA. This poster investigates alternative methods of calculating the SLA from mapped ESSs to reduce bias towards patchy and irregular areas of snow cover.

How to cite: Hallford, M., Rea, B. R., Spagnolo, M., Sam, L., Singh, S., and Mullan, D.: Calculating Snowline Altitudes on Glaciers with Patchy and Irregular Snow Cover Using Satellite Imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19873, https://doi.org/10.5194/egusphere-egu26-19873, 2026.

EGU26-20460 | Posters on site | CR1.1

Untangling multi-annual to decadal ice mass loss of glaciers in the Patagonian Andes 

Christian Sommer, Moritz Koch, Franziska Temme, Antonia Warnstedt, and Matthias Braun

The Patagonian Andes host the largest glacierized area in the Southern Hemisphere outside Antarctica and play a key role in regional freshwater resources and global sea-level rise. Meltwater discharge from Patagonian glaciers contributes to sea-level rise, while changes in freshwater runoff threaten downstream ecosystems and water availability. In particular, the Northern Patagonian Icefield (NPI), Southern Patagonian Icefield (SPI), and Cordillera Darwin Icefield (CDI) are vast temperate ice bodies and rank among the Earth`s mountain regions with the highest glacier mass-loss rates.

Here, we present new observations of glacier mass change across the Patagonian Andes for the period 2000–2025. We combine multi-mission remote sensing data, including synthetic aperture radar (SAR) digital elevation models (DEMs) from the TanDEM-X mission and satellite altimetry from CryoSat-2 and ICESat-2, to derive glacier-specific and regional geodetic mass changes. In addition, we account for ice mass loss committed by frontal ablation by estimating subaqueous volume change of lake- and marine-terminating glaciers from observed terminus retreat and ice thickness reconstructions.

Comparison with climate observations reveal a region-wide warming trend since the beginning of the 21st century. However, regional glacier mass change exhibits pronounced spatial and temporal heterogeneity. NPI glaciers show a marked acceleration in mass loss after 2013, while at SPI mass loss rates remained comparatively stable until 2019, after which annual mass loss increased to levels similar to the NPI. Similarly, the CDI exhibits a distinct increase in mass loss in recent years, after a short intermediate period of mass loss deceleration. Glacier-specific analyses of surface elevation change and ice flow velocity at major outlet glaciers reveal enhanced surface lowering and increased flow speeds near glacier termini over the past decade, due to intensified dynamic thinning. The observed regional and temporal variability in glacier response is likely linked to previously reported variations in precipitation and snowfall amounts. Overall, annual specific mass loss of the NPI and SPI since 2019 (~ -1.5 m w.e./a) has increased by more than 50% compared to the early 2000s (~ -1.0 m w.e./a).

How to cite: Sommer, C., Koch, M., Temme, F., Warnstedt, A., and Braun, M.: Untangling multi-annual to decadal ice mass loss of glaciers in the Patagonian Andes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20460, https://doi.org/10.5194/egusphere-egu26-20460, 2026.

EGU26-1661 | Posters on site | CR1.2

Cryospheric change and ecological security 

Yulan Zhang

Cryosphere mainly distributes in polar and high-altitude regions, which includes glaciers, ice sheets, sea ice, lake & river ice, permafrost & sub-sea permafrost, and so on. Under the ongoing climate warming, the cryosphere has been shrinking at an accelerating rate. Most of glaciers retreat and lose their mass loss. The active layer of permafrost deepens and soil temperature rises. All these changes have profoundly altered the regional or even global hydrology and water quality, and further act on the feedbacks to climate change. Besides, the rapid cryospheric changes are also reshaping the terrain and landforms. This is also closely related to the stability of the ecosystem. Meanwhile, cryosphere contains large of chemicals as “pool”, such as carbon, nitrogen, mercury and other pollutants, making it an important linkage for the global biogeochemical cycles, posing potential risks on the cryosphere ecological security.

How to cite: Zhang, Y.: Cryospheric change and ecological security, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1661, https://doi.org/10.5194/egusphere-egu26-1661, 2026.

EGU26-1802 | ECS | Orals | CR1.2

The Hidden Threat of Glacier Melt: Rising Mercury Levels in French Alpine Lakes 

Davide Mattio, Stéphane Guedron, Pierre Sabatier, Aurélien Dommergue, Antonio Martínez Cortizas, Antoine Rabatel, and Hélène Angot and the EPOCH ALPS team

The melting rate of glaciers in Europe has accelerated continuously since the 1980s and continues today at an unprecedented pace. Such rapid and sustained glacier retreat has important implications for the release of legacy contaminants stored in ice. Since the onset of the Industrial Revolution, atmospheric deposition has led to the accumulation of pollutants, including mercury (Hg)—a highly toxic element with well-documented impacts on ecosystems and human health—within glaciers. Ongoing climate-driven melting can remobilize these long-term contaminant reservoirs.
To investigate this process, we examined Hg accumulation rates (Hg AR) in sediments from two neighboring high-altitude lakes in the French Alps. One lake represents a reference system receiving only atmospheric inputs, while the other is influenced by both atmospheric deposition and meltwater from a shrinking glacier. Comparing the two sedimentary records allowed us to isolate the signal associated with cryospheric change.
In the reference lake, Hg AR is controlled by regional atmospheric Hg emissions and follows the expected anthropogenic pattern, with maxima during World War II and in the 1970s, followed by a steady decline in recent decades. In contrast, the glacier-fed lake shows a steadily increasing Hg AR from the early 1900s to the present, with a doubling of accumulation rates over the past several decades.
Using estimates of glacier volume loss over the last 50 years together with Hg concentrations in glacier ice and cryoconite reported in the literature, we demonstrate that the recent acceleration of Hg AR is consistent with enhanced Hg release driven by glacier shrinkage. These results indicate that glacier melt represents an additional and climate-sensitive source of legacy Hg to downstream aquatic systems, compounding the environmental impacts of cryospheric change alongside pressures such as freshwater scarcity.

How to cite: Mattio, D., Guedron, S., Sabatier, P., Dommergue, A., Martínez Cortizas, A., Rabatel, A., and Angot, H. and the EPOCH ALPS team: The Hidden Threat of Glacier Melt: Rising Mercury Levels in French Alpine Lakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1802, https://doi.org/10.5194/egusphere-egu26-1802, 2026.

EGU26-1956 | ECS | Orals | CR1.2

The impact of climate change on mid-latitude Mediterranean glaciers over the past 75 years 

Bingdian Wang, Philip Hughes, Christopher Darvill, and Jamie Woodward

Glaciers are sensitive indicators of climate change, yet only a small number that remain in the Mediterranean region. Of these, most have retreated well into cirques, persisting as small, isolated glaciers or ice patches. The climatic drivers of glacier and snowpack changes across the Mediterranean mountains over the past 75 years are assessed using temperature, precipitation, snow cover, and glacier mass balance data. Summer temperatures in the Mediterranean region have risen dramatically since the 1970s with the average increasing by >1.9 °C by 2024 relative to the 1991–2020 mean. Winter precipitation in the Mediterranean region has shown a slight decline over the last 75 years. From 2019 to 2023, snow cover duration declined across most of the Mediterranean. Regression analysis indicates that the North Atlantic Oscillation (NAO) exerts only a limited influence on glacier mass balance and snowpack variability in the Mediterranean. This is because the dominant control on mass balance change in the Mediterranean is summer temperature rather than precipitation, much more so than further north in Europe where NAO has more influence on glaciers. Despite this strong temperature sensitivity, some Mediterranean glaciers persist due to favourable local topoclimatic conditions. In particular, enhanced snow accumulation from snow avalanching and windblown snow compensates high summer ablation, highlighting the key influence of local topoclimatic conditions on glacier survival in the Mediterranean region. Although Mediterranean glaciers are sustained by high accumulation, they are strongly affected by summer temperature variability, reflecting the broader global pattern whereby warm–wet glaciers show greater temperature sensitivity than cold–dry glaciers. Understanding how glaciers and snowpack respond to climate change in the Mediterranean mountains has relevance beyond this region and provides an important comparison for other mid-latitude regions, such as the Alps, the Caucasus, and the Tibetan Plateau, where glaciers and snowpack are crucial for water supply.

How to cite: Wang, B., Hughes, P., Darvill, C., and Woodward, J.: The impact of climate change on mid-latitude Mediterranean glaciers over the past 75 years, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1956, https://doi.org/10.5194/egusphere-egu26-1956, 2026.

EGU26-3156 * | Orals | CR1.2 | Highlight

The second highest tsunami ever recorded 

Dan Shugar, Katherine Barnhart, Mira Berdahl, Jacqueline Caplan-Auerbach, Göran Ekström, Aram Fathian, Marten Geertsema, Stephen Hicks, Bretwood Higman, Erin Jensen, Ezgi Karasözen, Patrick Lynett, John Lyons, Thomas Monahan, Gerard Roe, Kristian Svennevig, Liam Toney, Maximillian Van Wyk de Vries, and Michael West

Over the past century, more than two dozen tsunamis with runups greater than 50 m have been reported. Of these, more than half were in the Arctic or subarctic, including the 1958 Lituya Bay megatsunami, which ran up 530 m in elevation. Many of those megatsunamis occurred in deglaciating fjords or valleys, and almost all were triggered by landslides. At 5:26 a.m. local time on 10 August 2025, a large landslide (>64x106 m3) collapsed about one vertical km onto South Sawyer Glacier and into Tracy Arm, a cruise ship-frequented fjord in southeast Alaska. The landslide triggered a megatsunami, which reached an elevation of 481 m up the opposite fjord wall before propagating out of the fjord into Stephens Passage and Endicott Arm to the south. The tsunami was experienced by multiple ships in the vicinity, but due in part to its early morning timing, luckily no deaths or injuries occurred.

 

The initial rock wedge failure transitioned into a rock avalanche as it traveled down the slope and produced globally observed long-period seismic waves equivalent in size to those of a M5.4 earthquake. The landslide was also preceded by more than 24 hours of microearthquakes attributed to slip along the failure surface, with increasing rate and amplitude until roughly an hour before failure. Long-period monochromatic global seismic signals persisted for over 36 hours. These signals are consistent with a landslide-induced seiche trapped in the fjord, an interpretation further confirmed by tsunami simulations and satellite observations.

 

The landslide and resulting hazard cascade was enabled by >6 km of retreat of South Sawyer Glacier since 1948, which we statistically attribute to anthropogenic warming. Most recently, the base of the failed slope was fully exposed between late June and early August 2025 when the glacier retreated several hundred metres. A large failure of a slope that had not previously been identified as a hazard, and with no precursory slope deformation, in a fjord with extensive recreational activity (e.g., cruise ships and personal pleasure craft) highlights the near-field risk of landslide tsunamis and underscores the importance of enhanced monitoring and continued research using a variety of tools, including seismic, remote sensing, and in situ monitoring.

How to cite: Shugar, D., Barnhart, K., Berdahl, M., Caplan-Auerbach, J., Ekström, G., Fathian, A., Geertsema, M., Hicks, S., Higman, B., Jensen, E., Karasözen, E., Lynett, P., Lyons, J., Monahan, T., Roe, G., Svennevig, K., Toney, L., Van Wyk de Vries, M., and West, M.: The second highest tsunami ever recorded, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3156, https://doi.org/10.5194/egusphere-egu26-3156, 2026.

The heterogeneous ablation rates of debris-covered glaciers strongly influence mass balance and melt patterns, yet the factors controlling this variability remain poorly understood. To understand this, this study quantifies ablation dynamics across the debris-covered zone of Panchinala A glacier, located in western Himalaya, India, using high-resolution unmanned aerial vehicle (UAV) photogrammetry data. Multi-temporal UAV surveys were conducted during ablation seasons of 2021 and 2022 to generate orthomosaics and digital elevation models (DEMs) at centimeter-scale resolution. Surface velocity was estimated using the More Global Matching algorithm implemented in the Ames Stereo Pipeline and combined with independent ice thickness estimates to compute flux divergence. Flow-corrected Lagrangian surface mass balance (SMB) was estimated using a continuity-equation approach, applying mass conservation under an assumption of constant ice density. During 2021–2022, the ablation area exhibited a mean horizontal velocity of 4.40 m a⁻¹; velocities decreased progressively along-flow toward the glacier front. The mean Lagrangian SMB across the ablation area was -602.6 kg m-² a-1 (2021–2022). The result indicates contrasting ablation patterns over ice cliffs and debris covered area. Ice cliffs and adjacent ablation hotspots (10 m buffer) contributed ~50% of total ablation while occupying ≤20% of the ablation area, whereas the remaining debris-covered surface (~80%) accounted for ~50%. These results show that high-resolution datasets are important for accurate surface mass balance estimation and for resolving the spatial heterogeneity of ablation on debris-covered glaciers.

How to cite: Godara, A. and Ramsankaran, R.: Quantifying Ablation Dynamics in the Debris-Covered Zone of Panchinala-A Glacier Using High-Resolution UAV Photogrammetry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3421, https://doi.org/10.5194/egusphere-egu26-3421, 2026.

EGU26-4464 | ECS | Posters on site | CR1.2

Quantifying frontal disintegration processes at Morteratsch-Pers glacier complex using high-resolution UAV imagery (2017–2025) 

Katarina Henning, Lander Van Tricht, Maaike Izeboud, Jonas van Breedam, Yoni Verhaegen, Leo Hoessli, Marin Kneib, Philippe Huybrechts, and Harry Zekollari

Glaciers in the European Alps are retreating and thinning rapidly due to increasing atmospheric temperatures with expected far reaching implications on water availability, biodiversity, and local economy. Given their critical role as freshwater reservoirs and climate indicators, monitoring glacier changes is essential. Uncrewed Aerial Vehicles (UAVs) provide high-resolution, cost-effective observations that bridge the gap between sparse field measurements and coarse satellite data, enabling detailed assessment of glacier surface dynamics. In this study, a UAV- derived high-resolution dataset spanning the years 2017 – 2025 is evaluated to study the frontal spatio-temporal dynamics of the Morteratsch-Pers glacier complex. Surface elevation and surface velocities are derived and combined with reconstructed ice thickness fields (based on radar measurements) to reconstruct the glacier surface mass balance over time. The results are then compared to in-situ stake observations to assess the influence of features such as debris cover and collapsing ice caves, not captured with the local measurements, on frontal retreat patterns.  

How to cite: Henning, K., Van Tricht, L., Izeboud, M., van Breedam, J., Verhaegen, Y., Hoessli, L., Kneib, M., Huybrechts, P., and Zekollari, H.: Quantifying frontal disintegration processes at Morteratsch-Pers glacier complex using high-resolution UAV imagery (2017–2025), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4464, https://doi.org/10.5194/egusphere-egu26-4464, 2026.

We use a three-dimensional time-dependent glacier model that couples higher-order ice flow dynamics with multi-dimensional englacial and supraglacial debris transport to investigate the behavior of debris-covered glaciers and their response to climate change. By applying the model to a synthetic idealized glacier, our simulations allow for multi-dimensional, physically-based and general insights into debris-ice interactions. The model incorporates a melt-modification parameterization based on a synthesis of Østrem curves from previous debris-covered glacier studies, which is coupled to submodules for the spatio-temporal evolution of debris. The debris submodule also includes an off-glacier debris evacuation scheme which allows our simulations to reach a steady state debris mass, while explicitly ensuring debris mass conservation. Results reveal that the presence of a debris cover significantly alters the steady state glacier geometry and dynamics, as well as its climate change response. Debris-covered glaciers in some specific environmental settings are also found to be prone to the formation of stagnant, isolated dead ice bodies during glacier recession. The results highlight the importance of representing a more complete and multi-dimensional set of key debris processes in debris-covered glacier models, including (i) a melt-modification curve that captures melt enhancement for thin debris, (ii) resolving dynamic debris-ice interactions in three dimensions with higher-order ice flow, (iii) explicitly modelling the multi-dimensional, spatio-temporal evolution of a supra- and englacial debris mass, and (iv) a mass-conserving debris off-loading procedure which allows the model to reach steady state. Our main findings therefore emphasize the need to incorporate robust debris modelling in future glacier projections.

How to cite: Verhaegen, Y. and Huybrechts, P.: Coupling debris transport to 3D higher-order ice flow dynamics to model the behavior and climate change response of debris-covered glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4500, https://doi.org/10.5194/egusphere-egu26-4500, 2026.

EGU26-6503 | ECS | Posters on site | CR1.2

A historical time series of glacial debris cover change in the Himalayas using multi-source satellite data and deep learning 

Katrina Lutz, André Wolf, and Matthias Braun

Accurate estimation of current and historical glacier area provides crucial information for glacier monitoring and for projecting future glacier change. Despite significant advances in remote sensing, automated glacier delineation techniques still exhibit limited accuracy in debris-covered areas, often requiring time-consuming manual corrections, which are impractical for widespread application. While some regions have rich historical records of glacial development due to ease of access and scientific prioritization, many regions are represented by only a few outlines.

The Himalayas contain many large and heavily debris-covered glaciers, whose retreat and increase in debris coverage could drastically affect the primary source of freshwater for many communities. This vast and important region, however, has very few harmonized and temporally consistent datasets available for scientific use. Existing inventories are generally derived from imagery acquired in different years and exhibit substantial differences in their debris-covered area outlines.

Thus, to improve on these inconsistencies and inaccuracies, we are creating a historical time series spanning the entirety of the Himalayas between 1984 and 2025 with two-year intervals. To overcome the difficulties inherent to debris-covered glacier inclusion, several data sources are used, including optical, infrared, thermal, spectral indices, elevation change rate, surface velocity, and topographic parameters. These data sources are trained on a deep learning network comprised of a pre-trained U-Net with a long short-term memory (LSTM) module, which enhances debris segmentation by introducing historical data to the training process. In addition, the potential benefit of including radar coherence data is evaluated to assess whether glacier outlines produced in recent decades can be further refined.

How to cite: Lutz, K., Wolf, A., and Braun, M.: A historical time series of glacial debris cover change in the Himalayas using multi-source satellite data and deep learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6503, https://doi.org/10.5194/egusphere-egu26-6503, 2026.

EGU26-6845 | ECS | Posters on site | CR1.2

The impact of supraglacial ice cliff and pond formation on debris-free, tropical glacier mass loss 

Owen King, Nilton Montoya, Bethan Davies, Tom Matthews, Miguel Vargas, Sajid Ghuffar, Tom Gribbin, Baker Perry, Maxwell Rado, Robert McNabb, Lindsey Nicholson, and Jeremy Ely

Tropical Andean glaciers provide an important flux of freshwater to communities living both in high-altitude Cordillera and population centres downstream in countries such as Peru and Bolivia. Glacier recession threatens the sustainability of these water resources, and accurate modelling of future glacier behaviour is required to manage water stress in the region. These models must capture all processes contributing significantly to overall glacier mass budgets. Here we examine supraglacial pond and ice cliff development on three clean-ice glaciers in the Cordillera Vilcanota, Peru and their overall contribution to glacier mass balance. Whilst such features are common and well-studied on debris-covered glaciers, their development on debris-free glaciers has not been examined in detail. We use high-resolution contemporary and historical satellite imagery and repeat drone surveys to examine surface structure and geometry change over three glaciers during 1977–2024. We show how cliff and pond formation is driven by aspect-dependent surface melt of crevasse walls. These features act as ice loss hotspots, which enhance glacier net mass loss by ∼10% despite accounting for <5% glacier surface area. Incorporation of such amplified ice loss processes should be a priority for glacier model advances to achieve more accurate projections of future tropical glacier recession.

How to cite: King, O., Montoya, N., Davies, B., Matthews, T., Vargas, M., Ghuffar, S., Gribbin, T., Perry, B., Rado, M., McNabb, R., Nicholson, L., and Ely, J.: The impact of supraglacial ice cliff and pond formation on debris-free, tropical glacier mass loss, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6845, https://doi.org/10.5194/egusphere-egu26-6845, 2026.

EGU26-6984 | ECS | Orals | CR1.2

Wavering Ways Waves Work: Understanding glacier ogive formation using satellite and field observations combined with modelling 

Naomi Ochwat, Yoram Terleth, Robert S. Anderson, Alison Banwell, Martin Truffer, Cal Hobson, Sydney Bidwell, Emma Neuhauser, and Julia Kaltenborn

Wave ogives are among the most striking and least studied glacier surface features. They sometimes form at the bottom of icefalls, yet exactly how they form has eluded scientists for decades. On the Gilkey Glacier, below the Vaughan Lewis Icefall in the Juneau Icefield region of Alaska there is a well-developed series of wave ogives. Our study uses geophysical field observations of the Gilkey Glacier ogives combined with satellite data and modeling to better understand the formation process. Satellite-derived DEMs provide ogive amplitudes of 5-8 m and wavelengths of ~130 m. By combining Global Navigation Satellite System (GNSS), satellite, and timelapse camera-derived velocity observations, we found that the Vaughan Lewis Glacier is significantly slower than the Gilkey Glacier (60 m/yr compared to 130 m/yr), and the icefall is exceptionally fast (~2200 m/yr). We used the velocity and ogive characteristics to constrain parameters in a finite-difference numerical model that simulates ogive formation. Using this model, we tested the plausibility of the two formation mechanisms; i) seasonal mass balance variation; and ii) seasonal velocity variation of the lower glacier. Our results suggest that seasonal velocity variation of the lower glacier is the primary driver in wave ogive formation.

How to cite: Ochwat, N., Terleth, Y., Anderson, R. S., Banwell, A., Truffer, M., Hobson, C., Bidwell, S., Neuhauser, E., and Kaltenborn, J.: Wavering Ways Waves Work: Understanding glacier ogive formation using satellite and field observations combined with modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6984, https://doi.org/10.5194/egusphere-egu26-6984, 2026.

EGU26-7722 | ECS | Orals | CR1.2

Modern palynological assemblages in fjord surface sediments: indicators of Greening Svalbard 

Mincheol Lee, So-Young Kim, Jung-Hyun Kim, and Eunji Byun

The Arctic is experiencing rapid climatic warming. The inflow of warm Atlantic Water through the Fram Strait is an additional forcing to the stability of the Arctic cryospheric system, with the Svalbard archipelago being especially sensitive to its primary influence. While recent studies show the “greening” of this region through remote sensing and field observations, this study investigates modern palynological assemblages from fjord surface sediments at 34 different locations in Spitsbergen and Nordaustlandet to explore where this phenomenon is prevalent at an ecosystem scale. Long-distance transported pollen such as Pinus and Betula are consistently identified across fjords, while various and local pollen compositions are observed more in Isfjorden where intensive human activity and substantial retreat of tidewater glaciers have been reported. In addition to herbaceous pollen taxa, shrub pollen including Salix and Dryas is present on the western side of the archipelago more often. During pollen identification, abundant testate amoebae were also detected at most locations. We propose the following explanation on the observed palynological assemblages. Overall, pollen records from the surface fjord sediments reflect terrestrial environmental conditions effectively and spatially. The exposure of newly deglaciated surfaces where soils develop, subsequent ecological succession on these soils facilitates Arctic shrubification. Soil development can be inferred from testate amoebae, and Arctic greening can be detected through local pollen spectra. In our future analysis, the onset of these modern palynological assemblages can be identified through the investigation of fjord long core sediments.

How to cite: Lee, M., Kim, S.-Y., Kim, J.-H., and Byun, E.: Modern palynological assemblages in fjord surface sediments: indicators of Greening Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7722, https://doi.org/10.5194/egusphere-egu26-7722, 2026.

EGU26-9610 | ECS | Posters on site | CR1.2

Assessing glacier mass sensitivity to climate variability using GRACE/-FO 

Louis-Marie Gauer, Etienne Berthier, and Alejandro Blazquez

In many mountain regions, glaciers constitute an essential freshwater reservoir and represent a critical water supply for downstream populations during droughts. Moreover, glacier mass changes provide a direct and valuable indicator of ongoing climate change. While long-term glacier mass loss is well documented, the drivers of temporal variability in regional glacier mass balance remain poorly constrained, despite their importance for understanding regional glacier–climate interactions.

Satellite gravimetry missions Gravity Recovery and Climate Experiment (GRACE) and GRACE Follow-On (GRACE-FO) provide direct observations of mass variations at monthly timescales with global coverage over the past two decades. Here, we use GRACE/-FO Level-3 products to estimate glacier mass changes over some regions of the Randolph Glacier Inventory (RGI v6.0) and to investigate their sensitivity to climate variability. Two GRACE/-FO solutions are considered: a solution based on Multichannel Singular Spectrum Analysis (M-SSA), and the SAGSA ensemble solution combining products from multiple processing centers. Signal leakage and separation effects related to the coarse spatial resolution of gravimetry are mitigated using geometry-based approaches, enabling regional mass balance estimates.

Monthly region-wide glacier mass balance are then used to explore relationships with key climate-related drivers, with an initial focus on near-surface air temperature and precipitation derived from the ERA5 reanalysis. This study aims to explore the links between glacier mass variability and climate-related drivers using GRACE/GRACE-FO observations.

How to cite: Gauer, L.-M., Berthier, E., and Blazquez, A.: Assessing glacier mass sensitivity to climate variability using GRACE/-FO, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9610, https://doi.org/10.5194/egusphere-egu26-9610, 2026.

EGU26-10641 | ECS | Orals | CR1.2

Past and future drivers of glacier mass changes in High Mountain Asia and their impacts on catchment hydrology 

Achille Jouberton, Thomas Shaw, Evan Miles, Main Kneib, Koji Fujita, and Francesca Pellicciotti

In High Mountain Asia (HMA), glaciers and seasonal snowpacks have seen a widespread decline in the last two decades. However, these changes have been highly heterogeneous: glaciers of the Pamirs and Karakoram have seen positive mass balances in the early 2000s but are now on a trajectory of decline, while moderate and rapid mass loss occurs in the Central Himalayas and southeastern Tibetan Plateau, respectively. To understand these contrasting behaviours, their future trajectory, and their impacts on streamflow, we combine several years of situ observations and climate reanalysis with highly resolved land-surface and ice-flow models. We simulate water fluxes from 1970 to 2100 across three catchments with contrasting climatic settings. The catchments are in the Northwestern Pamirs (Kyzylsu), Central Himalayas (Trambau-Trakarding), and Southeastern Tibetan Plateau (Parlung No.4), spanning elevations from 2100 to 6800 m a.s.l.. 

We simulate the largest mass loss acceleration at Parlung No.4 Glacier, from  -0.10 m w.e. yr-1 in 1970-1999 to -0.80 m w.e. yr-1 in 2000-2023. The limited mass loss at Kyzylsu in 1970-1999 accelerated after 2000, mostly driven by a rapid worsening of glacier health in 2018-2024 (-0.72 m w.e. yr-1). Mass loss remained moderate at Trambau-Trakarding, from -0.39 m w.e. yr-1 in 1970-1999 to -0.30 m w.e. yr-1 in 2000-2023. 

These heterogeneous glacier mass balance patterns were driven by different summer 0°C isotherm changes, and contrasting precipitation decadal variability. Our projections forced with downscaled CMIP6 show that continued warming will expand ablation areas and extend melting into former accumulation areas previously located above the freezing line. On-glacier summer snowfall is projected to decrease by up to 60% by 2100 due to changes in precipitation phase. However, this will largely be offset by increases in snowfall in other seasons, driven by the widespread rise in precipitation projected for HMA. Despite stable accumulation rates, enhanced melt will drive severe glacier volume loss, strongly reducing the likelihood of new prolonged periods of near-stable or positive mass balances seen in our 1970-2020 simulations. 

Glacier retreat, combined with snowline rising to 6000 m a.s.l., will shift meltwater generation to higher elevations, where mass turnover rates will intensify. High-elevation areas will maintain their role as water providers, but with diminished capacity for water storage. We find that the evolving runoff contributions can decouple catchment-scale peak water from glacier-scale peak water. Indeed, substantial increases in rainfall (from 49 ± 22 % at the catchment in the Pamirs to 290 ± 146 % in the southeastern Tibetan Plateau), caused by precipitation phase and amount changes, and relatively stable snowmelt compensate for ice-melt reduction and postpone the timing of maximum runoff. While we find that ice melt nears its peak at Kyzylsu, with considerable uncertainty due to the initial ice volume, we project catchment runoff to continue increasing at all sites until the end of the century. Our results highlight the importance of considering the glacier 'peak water' concept within a catchment or basin hydrological framework.

How to cite: Jouberton, A., Shaw, T., Miles, E., Kneib, M., Fujita, K., and Pellicciotti, F.: Past and future drivers of glacier mass changes in High Mountain Asia and their impacts on catchment hydrology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10641, https://doi.org/10.5194/egusphere-egu26-10641, 2026.

EGU26-10843 | ECS | Posters on site | CR1.2

Modelling the Future of Indus Glacier Water Resources: Interactions between Glacier Retreat and Water Demand 

Alexandra von der Esch, Lander van Tricht, Matthias Huss, Marit van Tiel, Marin Kneib, Justine Berg, and Daniel Farinotti

Glaciers in the Indus are critical water resources, supporting agriculture, hydropower, and livelihoods for hundreds of millions of people downstream, especially during the dry season. Here, we assess changes in the future water availability from melting glaciers in the Indus basin and how this will impact future water scarcity risks. We model the evolution of all glaciers, in the Indus, larger than 0.5kmusing the Global Glacier Evolution Model (GloGEM), calibrated with transient snowline altitudes and geodetic mass balance observations. Glacier runoff projections are combined with water demand simulations from the ISIMIP3b dataset on total potential water withdrawal allowing us to explore potential future risks of water scarcity under SSP1-2.6 and SSP5-8.5 scenarios.

We analyse two different scenarios: (i) future changes in glacier runoff with present-day (2001-2020) water demand held constant, (ii) concurrent changes in both future glacier runoff and water demand. Preliminary results show that ongoing glacier mass loss in the Indus basin substantially changes the magnitude and seasonal distribution of glacier runoff. Timing of  peak seasonal ablation is shifted by up to several weeks, and the overall amount of glacier runoff is reduced, which has implications for downstream water availability, particularly during the early and late summer months, when demand is highest. By disentangling the contribution of glacier runoff to water demand, this study aims to quantify the vulnerability of the Indus to future water stress and to identify conditions under which glacier retreat may exacerbate or temporarily mitigate water scarcity. 

How to cite: von der Esch, A., van Tricht, L., Huss, M., van Tiel, M., Kneib, M., Berg, J., and Farinotti, D.: Modelling the Future of Indus Glacier Water Resources: Interactions between Glacier Retreat and Water Demand, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10843, https://doi.org/10.5194/egusphere-egu26-10843, 2026.

EGU26-11322 | ECS | Posters on site | CR1.2

Modelling subsurface melt of Swiss glaciers 

Leo Hösli, Matthias Huss, and Daniel Farinotti

Glacier subsurface melt, consisting of englacial and basal melt, is far less understood than surface mass balance. Yet it represents a potentially relevant component of glacier retreat dynamics. Research on subsurface melt has been limited due to scarce observations and incomplete process understanding.

Here, we quantify spatially distributed subsurface melt of Swiss glaciers using a modelling approach, constrained and validated by field observations. To constrain the model, we use field data on energy content of subglacial water and airflow collected at 5 individual glaciers. This included water temperature and discharge measurements of ice-marginal, subglacial, supraglacial and proglacial streams, as well as measurements of melt and air flow inside ice caves. To acquire validation data on subsurface melt rates, vertical ice motion of ablation stakes was measured on the glacier terminus of two glaciers using differential GPS. After correcting for advection and ice flow divergence, residual vertical ice motion was assumed to be equivalent to subsurface melt. The parameterized subsurface melt model is based on sub- and englacial energy exchanges and uses surface mass balance, glacier geometry, catchment topography, and weather data as primary inputs. Subsurface melt is represented through several components: (1) geothermal heat flux, (2) frictional and strain heating, (3) potential energy release from meltwater, (4) advection of energy from ice-marginal and supraglacial streams, and (5) airflow through subglacial channels. To model the spatial distribution of subsurface melt we use spatially distributed surface mass balance, flow routing, and assumptions on energy exchange between subglacial water and ice.

Model results indicate that the dominant contribution to subsurface melt comes from energy input by ice-marginal streams, followed by potential energy release of meltwater. Glacier-wide annual subsurface melt rates averaged across Swiss glaciers are in the order of tens of mm w.e. a-1, with larger glaciers generally exhibiting higher subsurface melt rates. Spatially, subsurface melt is highest near glacier termini, reflecting the location of ice-marginal stream inflow. A high elevation gradient (potential energy release) and a larger glacier area (larger catchment for ice-marginal streams) were identified as key controls on elevated subsurface melt rates. Validation data were found to be of the same order of magnitude as modelled values at the two respective field sites.

These results demonstrate that subsurface melt can be quantified using a combination of direct field observations and spatially distributed modelling. By providing spatially resolved estimates of subsurface melt for Swiss glaciers, this approach allows subsurface processes to be better understood and explicitly included in glacier evolution models. This constitutes an important step towards a more comprehensive and physically consistent description of glacier mass balance under ongoing climate change.

How to cite: Hösli, L., Huss, M., and Farinotti, D.: Modelling subsurface melt of Swiss glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11322, https://doi.org/10.5194/egusphere-egu26-11322, 2026.

EGU26-11770 | Posters on site | CR1.2

Dataset Discrepancies Dominate Present and Future Precipitation-Glacier Relationships Across High Mountain Asia 

Thomas Shaw, Achille Jouberton, Marin Kneib, Evan Miles, Masashi Niwano, Koji Fujita, Pascal Buri, and Francesca Pellicciotti

High Mountain Asia (HMA) provides crucial water resources to more than 1.5 billion people and accurate quantification of high elevation precipitation in this region is essential for understanding the hydrological cycle, patterns of ongoing climatic change, and water resource management. This is particularly the case in high elevation, glacierised catchments where the interplay of cryospheric and atmospheric processes limits our understanding of current and future water resource availability. The role of precipitation and snow accumulation is critical for the health of glaciers which represent both an important freshwater storage and hydrological buffer to drought conditions. In both present-day and future modelling scenarios, precipitation at both macro and local scales generate some of the greatest uncertainties in glacier response to climate, especially across the distinct hydro-climatic regions of HMA.

 

We leverage precipitation estimates across several regional gridded products with a high spatial (>= 10 km) and temporal (hourly) resolution to explore their discrepancies over glacierised regions of HMA for the period of 2001-2019. Our analyses demonstrate a substantial disagreement between precipitation datasets in terms of i) their annual and seasonal magnitudes, ii) the fraction of precipitation occurring during the summer/monsoon period, iii) the differences of precipitation amounts between decades, iv) the correlation of precipitation amounts to annual mass balances, v) diurnal precipitation frequency and, vi) dependence on elevation and topographic complexity. 

 

Using the Open Global Glacier Model (OGGM), we demonstrate that the selection of precipitation input data can lead to widely differing interpretations of the role of precipitation as a driver of mass balance variability under a future climate and create substantially different estimations of runoff that exceed the differences due to the choice of climate model.

At catchment scales, the spatial extent and seasonality of precipitation, as well as the representation of specific storm events are all critical for the accurate estimation of glacier energy and mass balance. Fully-physical modelling of well-monitored, glacierised catchments across HMA reveals that the timing of precipitation events can be equally important to the long-term mass balance of glaciers as the monthly amounts of precipitation from different datasets.  

Finally, we discuss the regions of greatest disagreement and highlight further investigations linking precipitation and glacier health under present and future climate.

How to cite: Shaw, T., Jouberton, A., Kneib, M., Miles, E., Niwano, M., Fujita, K., Buri, P., and Pellicciotti, F.: Dataset Discrepancies Dominate Present and Future Precipitation-Glacier Relationships Across High Mountain Asia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11770, https://doi.org/10.5194/egusphere-egu26-11770, 2026.

EGU26-13133 | ECS | Posters on site | CR1.2

Four decades of pan-Arctic glacier calving fluxes from multimodal satellite imagery 

Tian Li, Fabien Maussion, and Jonathan Bamber

The Arctic has been warming four times faster than the global mean over the last forty years. In response, the mass loss of glaciers has been accelerating and contributing to global sea-level rise. However, many of the mechanisms of this mass loss process are not well understood, especially the calving dynamics of marine-terminating glaciers, in part due to a lack of high-resolution calving front observations. To address this limitation, we developed a novel automated deep learning framework to automatically detect calving fronts in multimodal satellite imagery, including optical and SAR satellite images from Landsat, Terra-ASTER, Sentinel-2, and Sentinel-1 missions. In total, this provides an approximately four-decade time series of calving dynamics across Arctic glaciers and ice caps. The method was tested and developed initially on the Svalbard archipelago, where we identified widespread calving front retreats during the past four decades, including attribution to climate forcing mechanisms. Here, we have extended the analysis across the entire Arctic to produce a time series that starts in the 1980s with quasi-annual temporal resolution, but achieves sub-monthly sampling from 2014 onward, following the launch of Sentinel-1. This provides both seasonal and inter-annual calving dynamics for almost all marine-terminating glaciers in the Arctic, which have been used to explore and understand the drivers of calving processes.

How to cite: Li, T., Maussion, F., and Bamber, J.: Four decades of pan-Arctic glacier calving fluxes from multimodal satellite imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13133, https://doi.org/10.5194/egusphere-egu26-13133, 2026.

EGU26-14057 | Orals | CR1.2

Taking a glimpse into the glacier demise of the European Alps – a 3D portrait 

Johannes Jakob Fürst, Oskar Herrmann, Alexander Raphael Groos, Mamta Kc, Veena Prasad, Christian Sommer, and Guillaume Jouvet

Glacier demise is palpable in mountain regions around the world. This retreat affects marine and terrestrial ecosystems, regional year-around water security as well as increases the risk for mountain hazards. Satellite remote sensing techniques have drawn a sinister picture of increasing rates of ice loss, particularly in the European Alps. There, model projections suggest that glaciers will largely disappear from the mountain landscape by the end of the century. Under most optimistic scenarios with a regional warming below ~3°C, one third of the ice volume can be preserved. Only the larger and more elevated ice bodies will survive. Most glaciers will however disappear. Here, we will redraw this picture combining 3D glacier evolution modelling with systematic data assimilation. In this way, a seamless record of glacier evolution in the European Alps is produced, spanning the time period 2000 to 2100 and considering various climate scenarios.  Its main asset is that no geometric simplifications are applied as typically done in current tools for regional glacier modelling. Together with inverse and ensemble techniques for data assimilation, our approach can directly ingest map products of observed surface velocities as well as the spatial pattern of the observed 2000-2020 elevation change. For our future projections, we exclusively rely on high-resolution regional climate models, better representing the atmospheric conditions over mountainous.

Our results largely corroborate the above-described grim fate for the European glacier population. The retreat is primarily driven by temperature increase rather than precipitation changes.  For the first time, 3D simulations make this retreat tangible in its full extent. Even under the most favourable climatic trajectories, glacier remnants will only survive as isolated ice patches at high altitudes. Like hermits or relicts from the past, they will have largely disappeared from the public perception in Central Europe - at the latest by 2100. We further break down our projections by Alpine sub-regions. We find more pronounced values of relative volume loss in southern and eastern regions (e.g., Rhaetian Alps). Regions with little coverage at present (e.g., Glarus Alps) will virtually become ice-free. Only exception is the French region of the Dauphiné Alps. In general, glaciers in the north-western ranges (Pennine, Bernese, Graian Alps) appear more resilient to future warming – as glacier there can retreat to higher altitudes.

How to cite: Fürst, J. J., Herrmann, O., Groos, A. R., Kc, M., Prasad, V., Sommer, C., and Jouvet, G.: Taking a glimpse into the glacier demise of the European Alps – a 3D portrait, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14057, https://doi.org/10.5194/egusphere-egu26-14057, 2026.

EGU26-14771 | Orals | CR1.2

Vegetated debris-covered glaciers and stagnating patterns in the Manaslu region of Nepal Himalaya 

Adina E. Racoviteanu, Alienor Fichant, Diego Cusicanqui, Neil Glasser, Roman Millan, Stephan Harrison, and Benjamin A. Robson

Glacier complexes in the Manaslu region of Nepal Himalaya have been experiencing only moderate mean area losses and geodetic mass balance since the 1970s (~ -0.26 % a-1, -0.17 ± 0.03 m w.e.a−1. Many debris-covered glacier tongues exhibit large amounts of supra-glacial vegetation and stagnating patterns. Here, we investigate these apparent patterns of stagnation of glacier systems in this area, specifically the prevalent vegetation development and the geomorphological characteristics of debris cover tongues. We use remote sensing-derived surface velocities derived from image cross-correlation (RGDyn open-source package) based on Landsat and Sentinel-2 time series combined with high-resolution declassified Corona imagery and Pléiades. Preliminary results indicate ~8 % supra-glacial vegetation coverage at a regional scale and general glacier slowdown with variable movement rates depending on glacier morphology and debris covered characteristics.

How to cite: Racoviteanu, A. E., Fichant, A., Cusicanqui, D., Glasser, N., Millan, R., Harrison, S., and Robson, B. A.: Vegetated debris-covered glaciers and stagnating patterns in the Manaslu region of Nepal Himalaya, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14771, https://doi.org/10.5194/egusphere-egu26-14771, 2026.

EGU26-14845 | ECS | Orals | CR1.2

Probabilistic calibration of glacier projections using data assimilation 

Yeliz A. Yılmaz, Kristoffer Aalstad, Gregoire Guillet, David Rounce, Brandon Tober, Ruitang Yang, Henning Åkesson, and Regine Hock

Global glacier mass loss is accelerating, yet considerable spread in projected glacier changes remains due to model structure, forcing, and parameter uncertainty. Most global glacier projections rely on relatively simple models where calibration approaches are essential to constrain uncertainty by using scarce observations. Probabilistic calibration strategies that help with quantifying uncertainities have recently incorporated into a limited number of global glacier models. As a next step, we suggest employing Bayesian data assimilation methods with untapped potential to integrate multi source observations (in-situ, satellite, reanalysis) when calibrating global glacier model projections.

Here, we present a probabilistic calibration framework for the Python Glacier Evolution Model (PyGEM) based on ensemble-based data assimilation. Two data assimilation techniques (PBS and AdaPBS) are used to calibrate mass balance parameters to constrain future projections of glacio-hydrological variables (surface mass balance and runoff) between 2015 and 2100 under four SSP climate scenarios across the Scandinavian region. In this work, we compare our calibration results with commonly used deterministic and probabilistic glacier model calibration algorithms which are already in use in PyGEM. Our probabilistic calibration framework based on data assimilation has the potential to quantify and disentangle uncertainties from climate forcing, model structure, and parameters. Better constrained and uncertainty-aware glacier models increases confidence in projections of future glacier change and their relevant impacts. This work paves the way for producing policy relevant global glacier projections and scenarios with their uncertainty estimates within the ERC-AdG GLACMASS project.

How to cite: Yılmaz, Y. A., Aalstad, K., Guillet, G., Rounce, D., Tober, B., Yang, R., Åkesson, H., and Hock, R.: Probabilistic calibration of glacier projections using data assimilation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14845, https://doi.org/10.5194/egusphere-egu26-14845, 2026.

EGU26-15272 | Posters on site | CR1.2

Toward Minimally Calibrated Physics-Based Glacier Mass Balance Modeling 

Valentina Radic, Hannah Phelps, and Christina Draeger

Glacier mass loss has accelerated globally in recent decades, yet many regional and global glacier models still rely on temperature-index melt formulations that limit physical realism and process attribution. Physics-based approaches, such as surface energy balance (SEB) models, can overcome these limitations but are challenging to apply at regional scales because they require climate forcing resolved at local scales. Global climate models and reanalysis products are known to perform poorly in complex mountainous terrain without downscaling and bias correction. In addition, albedo parameterizations in SEB models typically require calibration against in-situ observations, which are sparse for most glacierized regions.


Here, we evaluate the skill of a physics-based glacier modeling framework designed to reconstruct glacier mass changes with minimal parameter calibration and without downscaling, and with only limited bias correction of climate input data. We first assess a relatively simple SEB model forced by climate variables from the European Centre for Medium-Range Weather Forecasts ERA5 reanalysis. Surface albedo, a key input to the SEB model, is prescribed using a standalone machine-learning model trained on Moderate Resolution Imaging Spectroradiometer (MODIS) satellite observations. We show that calibration of selected model parameters—most notably precipitation correction and albedo bias correction—is required for the model to perform well from local to regional scales across western Canada. We then evaluate a more complex SEB formulation using the open-source COupled Snowpack and Ice surface energy and mass balance model in PYthon (COSIPY), with the aim of assessing whether parameter calibration can be further reduced or avoided. We find that neural-network-based albedo estimates substantially improve model performance and that calibration-dependent albedo bias correction is no longer required when Landsat data are used instead of MODIS. In contrast, wind speeds from ERA5 require bias correction to obtain realistic turbulent heat fluxes, highlighting the importance of improving the representation of katabatic winds over glacier surfaces. With these adjustments, the non-calibrated physics-based model performs well in simulating summer mass balance at the glacier scale, provided that snow accumulation at the onset of the melt season is adequately captured. 

How to cite: Radic, V., Phelps, H., and Draeger, C.: Toward Minimally Calibrated Physics-Based Glacier Mass Balance Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15272, https://doi.org/10.5194/egusphere-egu26-15272, 2026.

EGU26-15329 | ECS | Posters on site | CR1.2

Modelling the Holocene evolution of Flade Isblink 

Alicia Bråtner, Mathieu Morlighem, Hélène Seroussi, and Shfaqat Abbas Khan

Understanding how ice caps and glaciers respond to climate change is essential for improving projections of present and future sea-level rise. The Holocene provides a valuable time period for this purpose, as it encompasses long-term ice–climate interactions and a transition from colder to warmer conditions comparable to today. 

Here we investigate the Holocene glacial history of the region presently covered by the Flade Isblink ice cap in northeast Greenland, a remote and high-elevation ice mass that is not directly connected to the Greenland Ice Sheet and is therefore particularly sensitive to climate forcing.

Flade Isblink is situated on the Kronprins Christian Land plateau and drains through fast-flowing outlet glaciers into the Arctic Ocean, storing a substantial volume of freshwater. Its geographic setting makes it an excellent indicator of Arctic climate variability. Here, we focus on identifying which parts of the ice cap survived the Holocene Thermal Maximum and on reconstructing ice extent in regions where geological constraints are sparse.

We use a two-dimensional coupled ice-flow and surface mass balance model implemented in the Ice Sheet and Sea-level System Model (ISSM) to simulate ice evolution from 12.4 ka BP to the present. Time-varying bedrock uplift and relative sea-level change are incorporated through an offline glacial isostatic adjustment (GIA) solution. To account for uncertainties in climate forcing, we run an ensemble of simulations spanning a range of climate scenarios. Model results are evaluated against geomorphological evidence, dated materials, and present-day ice geometry.

How to cite: Bråtner, A., Morlighem, M., Seroussi, H., and Khan, S. A.: Modelling the Holocene evolution of Flade Isblink, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15329, https://doi.org/10.5194/egusphere-egu26-15329, 2026.

EGU26-15852 | Orals | CR1.2

Heat wave events and the response of glaciers in the subtropical Andes 

Claudio Bravo, Alvaro Gonzalez-Reyes, Deniz Bozkurt, and Sebastián Cisternas

In recent decades, an increased frequency of heat waves (HWs) has been detected along the subtropical Andes (SA); however, their impact on the cryosphere has not been assessed in detail. Here we present a multi-scale assessment with the objective of quantifying the impact of HWs on Andean glaciers located in the SA. Sub-daily observations of melt at the Universidad (34°S) and Pichillancahue (39°S) glaciers show that the daily melt rate increases by approximately 25% during HW events compared to the rest of the ablation season. At the annual scale, the relationship is complex. Using seasonal HWs climatologies derived from the ERA5 reanalysis and glacial mass balances available from the World Glacier Monitoring Service (WGMS), it was determined that there is no significant relationship between the number of HW events and the annual mass balance. However, the annual mass balance of the Echaurren Norte Glacier (33°S) showed significant positive correlations (p<0.05) with the number of HW events occurring over the Pacific Ocean, during the spring and summer seasons between 1975 and 2023. Furthermore, the mass balance of the Piloto Este Glacier (33°S) also shows significant positive correlations with the number of HW events in the Pacific during spring and summer between 1979 and 2002. These correlations would indicate the importance of the higher evaporation rate during HW events, with the consequent contribution of moisture to the atmosphere, contributing to precipitation and snow accumulation on glaciers during synoptic events occurring over the Andes. The above is consistent with the fact that glaciers in the central Andes of Chile and Argentina are more sensitive to precipitation variability, as well as its relationship with the El Niño-Southern Oscillation (ENSO). While melt rates increase during HW events, the forcing  of evaporation rates during HW events over the Pacific would generate a greater impact on the annual glacier mass balance. This finding, from a glaciological perspective, calls for further investigation into the role of HW events over the oceans as drivers of evaporation and their transport and circulation mechanisms. This work is funded by the FONDECYT Iniciación Project 11240379.

How to cite: Bravo, C., Gonzalez-Reyes, A., Bozkurt, D., and Cisternas, S.: Heat wave events and the response of glaciers in the subtropical Andes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15852, https://doi.org/10.5194/egusphere-egu26-15852, 2026.

EGU26-15904 | Orals | CR1.2

Meltwater chemistry at two rapidly retreating Arctic Sweden glaciers: Implications for downstream nutrient supply in a warming climate 

Alicia Rutledge, Jeff Havig, Briony Horgan, Mark Salvatore, Candice De Anda, and Ian Marrs

The cryosphere is experiencing rapid decline due to climate change, with 25-54% mass loss of the world’s glaciers predicted over the next century. These changes have far-reaching implications including impacts on local geohazards, regional freshwater availability, global sea-level rise, and downstream nutrient supply. Though many studies have examined the physical processes associated with glacier change, we still lack a complete understanding of the associated geochemical consequences. This is especially important to constrain as glaciated catchments are important sources of lithogenic nutrients due to mechanical and chemical weathering, and meltwater transport in turn influencing downstream ecosystems.

To better constrain the effects of subglacial weathering on glacial runoff chemistry, water and ice samples were collected at Storglaciären and Isfallsglaciären, two polythermal glaciers in the Tarfala Valley, Arctic Sweden in the summers of 2024 and 2025. These glaciers have experienced dramatic thinning and retreat for the past century, with this trend recently accelerating. Water temperature, conductivity, pH and other parameters were measured in situ. Samples were analyzed for major and trace ion concentrations, total carbon, and stable water isotopes. These are the first reported geochemical measurements of this kind for the reference glacier Storglaciären.

Aqueous geochemistry results indicate that chemical weathering of the bedrock is likely driven by a combination of both carbonic (H2CO3) and sulfuric (H2SO4) acid dissolution, resulting in major cations (e.g., Ca, Mg), Si, and Fe being released from subglacial sediment. Solute concentrations are highest at the cold-based ice margins, indicating increased dissolution of Fe- and Mg-rich bedrock in these areas. Concentrations of sulfate are also highest under the cold ice, most likely due to increased FeS2 oxidation at the cold-based margins of the glacier.

These results indicate that heterogeneous oxidation most likely drives acidic weathering in the subglacial environment, and that this process appears to be more effective in the more stable, cold-based margins of the glacier where residence times of sediment are longer. Localized silica precipitation is more prevalent in the warm-based portions dominated by subglacial meltwater, glacial sliding, and seasonal flushing of sediment and water. These results suggest that there may be detectable differences in alteration processes between cold- and warm-based glacial thermal portions of ice sheets and glaciers, that these differences are detectable in local meltwaters, and that significant amounts of solutes are generated by subglacial alteration processes and transported to lower elevation Arctic ecosystems. It is imperative that future studies include repeat meltwater monitoring at these rapidly changing systems to understand the ongoing effects of climate change on glacial water chemistry and downstream nutrient supply.

How to cite: Rutledge, A., Havig, J., Horgan, B., Salvatore, M., De Anda, C., and Marrs, I.: Meltwater chemistry at two rapidly retreating Arctic Sweden glaciers: Implications for downstream nutrient supply in a warming climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15904, https://doi.org/10.5194/egusphere-egu26-15904, 2026.

EGU26-16470 | Posters on site | CR1.2

Changes in glacier runoff in a warming Arctic: simulations from the Bayelva catchment, Svalbard 

Thomas V. Schuler, Louise S. Schmidt, Maiken K. Revheim, and Sebastian Westermann

The Svalbard archipelago (76-81N) is undergoing increased warming compared to the global mean, which has major implications for freshwater runoff into the oceans from seasonal snow and glaciers. Quantifying changes of freshwater runoff  requires close integration of observations and process-based models.

Here, we use land-surface and ice-flow modelling in combination with satellite and in-situ observations, to simulate runoff from the Bayelva catchment, Svalbard (~30 km2, ~54% glacier cover), for the period 1991–2100. Runoff from seasonal snow and glaciers is simulated using the land surface model CRYOGRID, which includes a coupled energy balance-snow/firn model. Historical simulations (1991–2024) are forced by downscaled CARRA reanalysis data and evaluated against in situ measurements and geodetic mass balance observations. Future simulations (2024–2100) are driven by temperature and precipitation trends derived from CORDEX projections under the RCP4.5 and RCP8.5 scenarios.

To account for feedbacks between surface mass balance and glacier geometry, the runoff simulations are coupled to the 3D glacier evolution model IGM. Sentinel-1 surface velocity observations are used to constrain glacier sliding, while observed surface elevation changes are used to evaluate simulated thickness changes and in situ ice-thickness measurements to evaluate the initial glacier geometry.

For continued warming, glacier melt will intensify, thus increasing runoff, but at a later stage, the reduction of glacier area due to retreat will offset this effect, giving rise to a peak in glacier runoff. The simulations indicate that runoff from the Bayelva catchment is likely to peak within the next two decades. Under the RCP8.5 scenario, both glaciers within the Bayelva catchment, Austre and Vestre Brøggerbreen, are projected to largely disappear by 2100, resulting in a transition from glacier-dominated to snow-dominated runoff.

How to cite: Schuler, T. V., Schmidt, L. S., Revheim, M. K., and Westermann, S.: Changes in glacier runoff in a warming Arctic: simulations from the Bayelva catchment, Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16470, https://doi.org/10.5194/egusphere-egu26-16470, 2026.

EGU26-16695 | Posters on site | CR1.2

Towards a physically based framework of cryokarst evolution for dynamic modelling of debris covered glaciers 

Andreas Vieli, Florian Hardmeier, Evan Miles, Marin Kneib, and Argha Banjeree

Cryokarst processes such as ice cliffs, ponds and collapsed subglacial cavities have been recognized to substantially enhance surface ablation on debris covered glacier surfaces. Existing flow models for debris covered glaciers, however, still largely ignore their effects, thereby limiting the related predictions and understanding of dynamic feedbacks. We propose here a process based conceptual framework that dynamically simulates the melt enhancing effect along the glacier and can be coupled to a flow-model.

We approximate the enhancing effect of cryokarst through a state variable of ice cliff area density (ICAD) and which is simulated over time and space along the glacier surface through production, advection and reduction. The production of ICAD is assumed to be driven by the processes of meltwater incision, pondsand crevassing through extensional flow; ICAD is then advected at the surface by ice-flow. Reduction in ICAD is simulated through a typical decay timescale related to debris redistribution and burial and, for crevasses, through compressional flow. The drainage of supraglacial streams to the glacier bed under tensile strain rates or through cut-and-closure allows to remove supraglacial discharge, thereby stopping ice-cliff production from supraglacial channel incision. In addition, ICAD growth from full thickness collapse of non-pressurized subglacial channel voids is parametrized through subglacial stream discharge and a threshold in ice overburden pressure. The parametrizations of the above processes are based on variables that are directly available in flow models for debris covered glaciers and encompass ice thickness, surface slope, flow speed, debris thickness and surface ablation. This framework of modelling ICAD evolution is coupled to a flowline model for debris covered glaciers that dynamically tracks debris thickness and then uses ICAD to incorporate melt enhancement relative to clean ice. The effects of including cryokarst processes and the related feedbacks are then investigated for a synthetic debris covered glacier geometry. Modelling results indicate an enhancement of glacier decay in a warming world and are compared to observed relationships of ice cliff area density to variables such as flow speed, surface slope and debris thickness.

How to cite: Vieli, A., Hardmeier, F., Miles, E., Kneib, M., and Banjeree, A.: Towards a physically based framework of cryokarst evolution for dynamic modelling of debris covered glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16695, https://doi.org/10.5194/egusphere-egu26-16695, 2026.

EGU26-16948 | ECS | Orals | CR1.2

Beneath the ice: Unravelling the Topography of a Deglaciated Earth (TOPO-DE) 

Thomas Frank, Ward van Pelt, David Rounce, Guillaume Jouvet, and Regine Hock

Glaciers distinct from the ice sheets in Greenland and Antarctica are experiencing accelerating retreat. Consequently, landscapes so-far hidden beneath the ice will emerge, yet their characteristics are poorly constrained by existing observations and models. At the same time, the subglacial topography itself controls retreat patterns and magnitudes. Hence, an improved representation of the glacier bed is key for improved future projections of glacier evolution. Here, we present a physically plausible map of subglacial topography for all >200,000 glaciers in the world, called Topography of a Deglaciated Earth (TOPO-DE). The map is constrained by an inverse modeling approach that relies on the higher-order Instructed Glacier Model (IGM), a wealth of surface observations, and automatic Bayesian calibration against thickness observations. We find a global glacier volume of 149±29 × 103 km3 (316±61 mm sea level equivalent) and a mean glacier thickness of 212 m. While the global total is consistent with previous work, regionally variable discrepancies highlight the differences between this study and previous reconstructions based on shallow ice-flow physics. The landscapes beneath the ice are characterized by a large potential to host future lakes, quantified as a combined potential lake volume of >3,000 km3, or 2% of the global glacier volume, and a potential areal lake coverage of the presently ice-covered lands of 6%. We show where previous studies produced unphysical bed features and compare that to solutions of our model. Our freely-available bed product offers new insights into landscapes emerging after glacier retreat and can serve as an input for future projections of glacier change and its consequences.

How to cite: Frank, T., van Pelt, W., Rounce, D., Jouvet, G., and Hock, R.: Beneath the ice: Unravelling the Topography of a Deglaciated Earth (TOPO-DE), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16948, https://doi.org/10.5194/egusphere-egu26-16948, 2026.

EGU26-17201 | ECS | Posters on site | CR1.2

From the Little Ice Age to the future: modelling the evolution of Schiaparelli Glacier, Tierra del Fuego 

Franziska Temme, Jorge Berkhoff, Oskar Herrmann, Lukas Langhamer, Ilaria Tabone, Ricardo Jaña, and Johannes Fürst

Glaciers in Patagonia and Tierra del Fuego remain among the least studied worldwide, despite experiencing pronounced mass loss over recent decades. Many glaciers in this region terminate in lakes or the ocean, making their evolution dependent on mass balance both directly controlled by climatic forcing at the glacier surface as well as dynamically controlled at the ice front. Recent studies demonstrate that warming air temperatures have increased surface melt rates significantly, suggesting climatic changes as the main driver for the observed losses. Climatically driven thinning can, however, trigger ice-dynamic instabilities, potentially amplifying glacier retreat.

To improve our understanding of the interaction of both components, climatic mass balance and glacier dynamics, we aim to establish a comprehensive modelling framework for Schiaparelli Glacier in Tierra del Fuego. Schiaparelli Glacier terminates in a proglacial lake that formed after recession in the 1940s. Ice thickness reconstructions reveal a potential overdeepening near the glacier front, which may lead to a self-accelerating ice-dynamic retreat once the glacier retreats into deeper water. This setting, combined with the availability of more than a decade of glaciological, meteorological and hydrological in-situ observations, makes Schiaparelli Glacier an attractive and exciting research target.

The aim of this study is to set up a modelling framework to simulate the evolution of Schiaparelli Glacier in the past and future, covering the Little Ice Age to the end of the 21st century. To do so, we will rely on the FROST framework (“Framework for assimilating Remote-sensing Observations for Surface mass balance Tuning”), which applies an Ensemble Kalman Filter to calibrate glacier-specific surface mass balance parameters using remote sensing observations. FROST is coupled to the Instructed Glacier Model (IGM) to capture the glacier dynamics. We further upgrade the surface mass balance scheme from a basic temperature-index model to a simplified energy balance model that explicitly accounts for solar radiation. Past glacier extents derived from moraine and tree-ring dating are used to validate the reconstructed glacier evolution of Schiaparelli Glacier.

How to cite: Temme, F., Berkhoff, J., Herrmann, O., Langhamer, L., Tabone, I., Jaña, R., and Fürst, J.: From the Little Ice Age to the future: modelling the evolution of Schiaparelli Glacier, Tierra del Fuego, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17201, https://doi.org/10.5194/egusphere-egu26-17201, 2026.

EGU26-17501 | ECS | Orals | CR1.2

Glacio-hydrological modelling of the Aletschgletscher catchment with evolving supraglacial debris since 1900 

Vicente Melo-Velasco, Thomas Shaw, Michael McCarthy, Catriona Fyffe, Evan Miles, José Manuel Muñoz Hermosilla, Adrià Fontrodona-Bach, Prateek Gantayat, Achille Jouberton, and Francesca Pellicciotti

Supraglacial debris partially covers more than 40% of Earth’s glaciers (excluding Antarctica) and, where present, acts as a major controlling factor for glacier melt. It can enhance melt when the layer is thin by reducing surface albedo (increasing the net radiative flux) and it reduces melt when it is thick by insulating the ice from the atmosphere (dampening the conductive heat flux). Accurately simulating the spatio-temporal evolution of debris over a glacier is still a challenge, because of diverse debris sources and mechanisms of transport on and within the ice that affect long-term debris cover evolution. Previous studies have investigated the evolution of debris from geomorphological and historical data or from debris-tracking ice dynamics modelling. These approaches, however, often do not capture the transient ice melt-debris thickness relationship under a changing climate. To date, no attempt has been made to couple the century-scale evolution of debris extent and thickness with a full surface energy-balance model to evaluate debris-melt feedbacks and assess their impacts on catchment-scale runoff generation.

We apply a distributed land surface-energy balance model to simulate the glacier evolution and surface hydrology of the Aletschgletscher catchment (including glaciated and ice-free areas) in the Swiss Alps from 1900 to 2023. We incorporate the evolution of supraglacial debris, constrained using historical topographic maps and recent debris thickness measurements. We evaluate the impact that time-evolving debris-cover extent and thickness has on the glacier mass balance and hydrology. We also compare results for Grosser Aletsch and Oberaletsch to demonstrate that increasing catchment debris cover influences catchment response to climate and glacier change.

Our results show that the contribution of sub-debris melt to runoff varied substantially over the last century. The catchment-wide sub-debris melt contribution increased until ~1945, then declined until today. However, trends differed between subcatchments. In the sparsely debris-covered Grosser Aletschgletscher, sub-debris melt reached its peak around 1940 (25–30% of total ice melt) before decreasing until present (same pattern as the entire catchment). In contrast, the highly debris-covered Oberaletsch shows a continuous increase, with recent values reaching 40–50% without a clear peak. The catchment trend is primarily explained by the evolution of debris cover on Grosser Aletschgletscher, combined with climate factors. Periods of expanding debris extent (~1910–1930 and ~1940–1965) initially increased the sub-debris melt contribution by enlarging the area where melt is enhanced by thin debris. Once debris area stabilised and average thickness increased (post-~1965), the stronger insulating effect reduced its relative contribution. An early rapid thinning of debris (~1910–1920) further enhanced early melt. Furthermore, climate warming has raised the 0°C isotherm, increasing melt in debris-free areas and thereby relatively reducing the proportion of melt occurring under debris. Therefore, the sub-debris melt contribution is affected by the combination between debris evolution and climate change. In a world with darkening glaciers, it is essential for glacio-hydrological models to consider evolving debris extent and thickness, and to incorporate feedbacks related to these changes, which substantially impact the surface energy balance, in order to accurately project future runoff from these catchments.

How to cite: Melo-Velasco, V., Shaw, T., McCarthy, M., Fyffe, C., Miles, E., Muñoz Hermosilla, J. M., Fontrodona-Bach, A., Gantayat, P., Jouberton, A., and Pellicciotti, F.: Glacio-hydrological modelling of the Aletschgletscher catchment with evolving supraglacial debris since 1900, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17501, https://doi.org/10.5194/egusphere-egu26-17501, 2026.

EGU26-17756 | Posters on site | CR1.2

Drivers and impacts of extreme events on Flade Isblink ice cap. 

Louise Sandberg Sørensen, Kirk Scanlan, Renée Fredensborg, Natalia Andersen, Rasmus Arildsen, Jonathan Kirby, and Mikkel Kruse

The Arctic is increasingly influenced by extreme events both in environmental forcing, and in the response in the cryosphere. Still, the mechanisms linking short-lived events in the different component of the Arctic system (atmosphere, land ice, ocean and sea ice) remain poorly understood. Within the  ESA-funded ARCTEX project we use a range of EO datasets and model outputs to identify extreme events and their impact on three different ice caps/ glaciers in the Arctic: The Flade Isblink and Austfonna ice caps and Nioghalvfjerdsfjorden outlet glacier.

Here, we present our findings over the Flade Isblink Ice cap in Northeastern Greenland. We present a comprehensive suite of EO-derived data sets over and around the ice cap, and wavelet analysis to identify extreme events, periodicity and regime shifts in these time series. One finding is the surge of Marsk Stig Bræ, which was initiated after 2021, and the subsequent response in the surface topography of the ice cap. We examine the potential drivers and consequences of this surge, with particular emphasis on the possible coupling between glacier dynamics, the drainage of a nearby subglacial lake, sea ice variability and ocean temperatures. Using a multi-sensor Earth Observation approach combined with regional climate model output, we analyse the temporal evolution of ice velocity, surface elevation, meltwater production, and subglacial hydrology from 2011 to 2025. This study demonstrates the value of integrated, high-temporal-resolution EO datasets for resolving rapid cryospheric change.

How to cite: Sandberg Sørensen, L., Scanlan, K., Fredensborg, R., Andersen, N., Arildsen, R., Kirby, J., and Kruse, M.: Drivers and impacts of extreme events on Flade Isblink ice cap., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17756, https://doi.org/10.5194/egusphere-egu26-17756, 2026.

EGU26-18086 | ECS | Posters on site | CR1.2

Ablation and dynamics of four ice cliffs on the partially debris-covered glacier tongue of Kanderfirn, Swiss Alps 

Ann Christin Kogel, Anna Zöller, Christoph Mayer, and Alexander Raphael Groos

Debris-covered glaciers influence the regional hydrological cycle by modulating glacier melt processes. One important control on melt variability on debris-covered glaciers are ice cliffs, which have been identified as melt hotspots, exhibiting ablation rates that far exceed those of the surrounding debris-covered area. As a result, they contribute disproportionately to total glacier mass loss. However, their dynamics and contribution to overall ablation have been quantified for only a few glaciers, mainly in the Himalaya. Quantifying and parameterizing ice cliff dynamics, including modelling frameworks, is needed to reliably project the future evolution of debris-covered glaciers in different mountain regions, as well as their water supply.

The aim of this study is to quantify ice cliff melt and backwasting rates in alpine settings, to generate a reference dataset for ice cliff model applications and to assess their relative contribution to total ablation. Ablation and dynamics of four ice cliffs were measured between 26 August and 19 September 2025 at the Kanderfirn. The Kanderfirn, a valley glacier in the Swiss Alps, was selected for this study as the tongue comprises both debris-covered and debris-free areas and, thus, enables the study of different ablation processes at the same site. Four ice cliffs representing the four cardinal orientations were selected to assess differences in melt and backwasting rates related to the ice cliff orientation, which are discussed in the literature. In total, eight stakes were installed at the four ice cliffs, with one stake drilled into the bare ice face of each cliff and a corresponding stake placed in the debris-covered area immediately above each cliff, to quantify the vertical, tangential and sub-debris melt rates as well as horizontal backwasting rates. Eleven additional stakes were installed at sites with varying debris thickness. Moreover, repeated UAV surveys were carried out to generate digital elevation models for the investigation of the geometric evolution of the ice cliffs over a one-month period. Finally, a surface energy-balance model was applied to model ice cliff and sub-debris ablation using the UAV-based digital elevation model and meteorological data from on- and off-glacier weather stations.

The in-situ results show clear contrasts in melt rates between ice cliff faces and the surrounding debris-covered area, as well as variability among ice cliffs with different orientations, including differences in backwasting rates. Two separate estimates of apparent vertical melt rate are derived from tangential melt measurements as well as from backwasting and sub-debris melt, combined with the slope angle. The close agreement between both results indicates consistent field measurements. The measurements and modelling provide valuable insights into the ablation and dynamics of ice cliffs on an Alpine glacier.

How to cite: Kogel, A. C., Zöller, A., Mayer, C., and Groos, A. R.: Ablation and dynamics of four ice cliffs on the partially debris-covered glacier tongue of Kanderfirn, Swiss Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18086, https://doi.org/10.5194/egusphere-egu26-18086, 2026.

EGU26-19367 | ECS | Orals | CR1.2

Constraining debris input to Oberaletsch Glacier using ensemble-based Lagrangian modelling 

José M. Muñoz-Hermosilla, Evan Miles, Michael McCarthy, Vicente Melo Velasco, Florian Hardmeier, Prateek Gantayat, Adrià Fontrodona-Bach, Guillaume Jouvet, and Francesca Pellicciotti

Debris-covered glaciers play an important role in alpine hydrology, yet the origin and transport pathways of debris within the glacier remain difficult to constrain. This is a major limitation in glacier evolution models, many of which have tended to ignore debris transient effects, especially for assessment of catchment hydrological processes. Supraglacial debris coverage is an integrated signal of debris supply, climate forcing, glacier geometry and debris physical properties, all of which vary in time, resulting in a complex inverse problem for model-based reconstructions.

Here, we apply the Instructed Glacier Model (IGM) with a newly implemented Lagrangian debris transport module combined with an ensemble of climate forcing, to explore constraints on debris input at Oberaletsch Glacier in the Swiss Alps. This framework allows debris particles to be tracked within a dynamically evolving glacier geometry and enables a likelihood-based assessment of inferred debris source regions across the ensemble. Rather than seeking a unique reconstruction, we identify spatially persistent and statistically robust seeding areas that are compatible with the observed historical evolution of debris extent derived from debris-cover maps for 1965, 1985, 1995, 2000, 2010 and 2015. These areas are identified by tracing debris particles backward from their final positions within the observed debris-covered zone to their upstream seeding locations.

Our results show that our inverse filtering strategy effectively identifies potential debris input zones that are primarily controlled by glacier dynamics and geometry. Notably, including or excluding the effect of debris on surface mass balance does not significantly alter the reconstructed debris extent in the ablation zone, highlighting the dominant role of ice flow in shaping supraglacial debris patterns at glacier scale. The reconstructed debris input patterns allow us to reproduce the observed historical evolution of debris extent and glacier geometry with good agreement. Debris extent matching between simulations and observations reaches around 80%, while the percentage of the total particles ending up in the target debris area remains above 70%. Ongoing work addresses the reconstruction of debris thickness, which is sensitive to both the debris weight (i.e. the assigned debris volume) prescribed for each particle and, crucially, the climatic forcing, requiring an iterative approach to capture the full transient characteristics of the glacier debris cover.

This study demonstrates that ensemble-based Lagrangian modelling provides a powerful framework to constrain debris input to glaciers. By explicitly coupling debris transport to the evolving glacier dynamics, this approach opens new perspectives for interpreting present-day debris cover and for projecting the future evolution of debris-covered glaciers under changing climatic conditions.

How to cite: Muñoz-Hermosilla, J. M., Miles, E., McCarthy, M., Melo Velasco, V., Hardmeier, F., Gantayat, P., Fontrodona-Bach, A., Jouvet, G., and Pellicciotti, F.: Constraining debris input to Oberaletsch Glacier using ensemble-based Lagrangian modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19367, https://doi.org/10.5194/egusphere-egu26-19367, 2026.

EGU26-19772 | ECS | Orals | CR1.2

Modelling the impact of an evolving supraglacial debris cover on the future evolution of glaciers in a changing climate 

Prateek Gantayat, Evan S Miles, Achille Jouberton, Jose Manuel Munoz, Vicente Melo Velasco, Adria Fontrodona Bach, Michael McCarthy, and Francesca Pellicciotti

Recent climate warming has increased the extent of debris cover on mountain glaciers. A thicker debris cover tends to shield the glacier surface from melting whereas a thinner/ patchy debris cover can amplify surface melting, with consequences for glacier dynamics and evolution. Most modelling studies that have estimated glacier evolution at a regional scale either a) do not consider the impact of debris cover at all or, b) assume a temporally static debris cover. Some major advances have been achieved in a recent study that accounted for the impact of evolving debris cover on future evolution of glaciers with an aerial extent > 1 km2 in High Mountain Asia; however, limitations remained related to the parameterised relationships between debris cover area and thickness changes. Alternatively, debris-explicit ice flow models exist, but are not suitable for  regional or global scales due to the data inputs and spin-up period. As such, a gap exists for an approach to model dynamic debris that is physics-based but simple to implement in large-scale glacier models.

 

To address this gap, we present a 1D numerical ice-flow model based on the Shallow Ice Approximation (SIA) that  includes coupled sub-modules which explicitly evolve the debris cover and thickness using principles of mass conservation and a degree day approach for estimating surface mass balance. It uses freely available data namely ERA-5 daily data of temperature and precipitation, glacier geodetic mass balances, historic satellite-derived supraglacial debris cover, glacier surface elevation and glacier surface velocities as inputs. The debris extent/thickness module is easily calibrated; dependent on the mass balance parameters and does not lead to the problem of equifinality of parameter sets.

 

We demonstrate the model over four debris-covered glaciers located in  the Central European Alps (Oberaletsch, Zmutt, Pasterze and Miage glaciers), where present-day debris thickness data are available. Results from the historic simulations show that the model was able to estimate the distribution of debris thickness within an RMSE ~ 0.07 m. In addition to that, the modelled evolution of the debris cover area fraction (i.e., the fraction of the glacier area covered by debris in a 10-m surface elevation band) was also in good agreement with that measured with maximum RMSE of ~8% per elevation band. The future evolution of these glaciers was carried out by forcing the ice-flow model with CMIP6 derived SSP2-4.5 and SSP5-8.5 climate scenarios, and highlighting the process of tongue detachment from headwall mass supply areas in the 21st century. Future simulations revealed that these test glaciers would be nearly completely covered with debris by the end of the 21st century with debris thicknesses becoming at least twice as compared to the present state. In addition to that, these glaciers are also expected to break into fragments with the tongues getting detached from the main glacier.  Overall, the coupled model is easy to apply, computationally fast and is currently being used to study the impact of an evolving debris cover on glacier evolution, in the Central European Alps, under different climate scenarios.

How to cite: Gantayat, P., Miles, E. S., Jouberton, A., Manuel Munoz, J., Melo Velasco, V., Fontrodona Bach, A., McCarthy, M., and Pellicciotti, F.: Modelling the impact of an evolving supraglacial debris cover on the future evolution of glaciers in a changing climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19772, https://doi.org/10.5194/egusphere-egu26-19772, 2026.

EGU26-21674 | ECS | Posters on site | CR1.2

Modeling Glacier Evolution Across Different Climatic Regions of High Mountain Asia 

Muzammil Hassan, Rijan Bhakta Kayastha, Gong Cheng, Mohan Bahadur Chand, and Javed Hassan

In High Mountain Asia (HMA), glacier meltwater plays a critical role in regulating seasonal river discharge and supporting water availability for populations living in mountainous and downstream regions. Observed acceleration in glacier mass loss over recent decades, together with projected future warming and changes in precipitation, is expected to modify the timing and magnitude of meltwater contributions, with significant implications for regional water security, sustainable development, and glacier-related hazards. To quantify glacier responses to climate change under different emission scenarios, we model glacier evolution across diverse climatic settings in HMA, including the Central Karakoram, Tibetan Plateau, and Central Himalaya. We use a MOno-Layer Higher-Order ice-flow model within the Ice-sheet and Sea-level System Model on an unstructured triangular finite-element mesh, locally refined at high spatial resolution (30–500 m) based on present-day observed surface velocities. We use a nonlinear Budd friction law and the basal friction coefficients are inferred using surface velocity observations from 2022. Surface mass balance (SMB) is computed using a temperature-index method that explicitly accounts for debris cover effects. The SMB model is calibrated against geodetic mass-balance estimates derived from stereo imagery (2000–2020) and validated using satellite altimetry observations (2003–2023). We simulate the glacier evolution from 2000 to 2100 under SSP1-2.5, SSP2-4.5, SSP3-7.0, and SSP5-8.5 using climate forcing from five global climate models (GCMs). Based on ensemble of all five GCMs, glaciers are projected to loose 10 ± 16% (SSP1-2.5) to 98 ± 2% (SSP5-8.5) of their mass by 2100, relative to 2000 across the regions. Among all studied region Monumaha Ice field and Purogangri Ice Cap on Tibetan Plateau exhibit a maximum mass loss of up to 70 ± 22 to 98 ± 2%. We find that on individual glaciers mass change debris cover play an important role, particularly in Central Karakoram region where debris cover delayed the mass loss by 15% by the end of 2100. One of the major takeaways for our study is that compared to earlier studies based on flowline models, our estimates show that glacier mass change differs significantly

How to cite: Hassan, M., Kayastha, R. B., Cheng, G., Chand, M. B., and Hassan, J.: Modeling Glacier Evolution Across Different Climatic Regions of High Mountain Asia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21674, https://doi.org/10.5194/egusphere-egu26-21674, 2026.

EGU26-21688 | Posters on site | CR1.2

The effect of debris supply on glacier evolution: sensitivities and challenges 

Florian Hardmeier, Evan Miles, José M. Muñoz-Hermosilla, Guillaume Jouvet, and Andreas Vieli

Debris on glacier surfaces has a strong effect on glacier melt and is currently expanding and thickening due to climate change. Several studies have applied coupled debris-ice dynamic modelling in order to simulate the evolution of debris-covered glaciers. However, many aspects within these dynamic systems remain poorly constrained, as data is scarce and processes are complex and interdependent. So far, most approaches focused on the simulation of the debris layer in the ablation area, but preceding processes of debris supply through gravitational processes and englacial debris transport are often represented based on simple assumptions or limited measurements and with unknown uncertainties. In this study, we address this issue by investigating how changes in the spatial distribution of debris supply affect down-glacier debris transport and debris cover.

For this, we apply a novel 3-dimensional coupled debris-ice dynamics model, implemented within the Instructed Glacier Model (IGM), that uses particle tracking to model englacial and supraglacial debris transport. In this approach, particles need to be seeded to initialize their entry into the glacier system. This involves the development of a framework to decide where and at what rate we seed these particles. We test several approaches and implement a scheme that automatically generates seeding locations based on local topography. In our experiments, we find that small differences in along-flow seeding location can have a strong impact on englacial transport paths, debris cover extent, and finally glacier extent. This reasserts the need to better constrain debris supply as an important part of the process chain if we want other aspects to be accurately represented in models.

How to cite: Hardmeier, F., Miles, E., Muñoz-Hermosilla, J. M., Jouvet, G., and Vieli, A.: The effect of debris supply on glacier evolution: sensitivities and challenges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21688, https://doi.org/10.5194/egusphere-egu26-21688, 2026.

EGU26-22641 | Posters on site | CR1.2

Identifing the debris-covered terminus for the Middle-West Rongbuk Glacier at the Mt. Everest in the Central Himalayas 

Qinghua Ye, Nauman Ali, Kaman Ghimire, Junbo Wang, and Liping Zhu

Debris-covered glaciers have been widely recognized in glacier runoff contributions and ice-rock disasters. It showed that debris-covered glaciers occupy about 27% glacierized region in the Central Himalayas. However, the delineation of debris-covered glaciers is still the bottleneck, which leads to high uncertainties in glacier change deteriorating our understanding of the hazard cascade from the collapse of rock and ice. Therefore, it is vital to provide the definitive margins of the debris-covered ice.

Here, we put forward a suitable method to locate the debris-covered glacier terminus of the Middle-West Rongbuk glacier based on multi-temporal surface elevation change data pairs from multi-source remote sensing data (such as DEM differencing, ICESat-2 laser altimetry, and InSAR technology). According to the DDh indicator (the difference in Dh), the debris-covered glacier terminus is determined. In addition, the glacial movement velocity generated from Sentinel-1 images was also used to verify the determined terminus outline of the debris-covered glacier. Our results showed that, from 1974 to 2025, the terminus of the debris-covered Rongbuk Glacier continuously migrated to higher elevations, rising from about 5240±20 m in the 1970s to 5290±20 m in the 2000s, then upward further to 5400±50 m after the 2010s. Over the past 48 years, the cumulative upward shift was approximately 160 m.

How to cite: Ye, Q., Ali, N., Ghimire, K., Wang, J., and Zhu, L.: Identifing the debris-covered terminus for the Middle-West Rongbuk Glacier at the Mt. Everest in the Central Himalayas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22641, https://doi.org/10.5194/egusphere-egu26-22641, 2026.

EGU26-22830 | Posters on site | CR1.2

Monitoring Argualas rock glacier dynamics combining InSAR, GNSS and UAV data 

Pablo Ezquerro, Jesús Revuelto, Juan López-Vinielles, Eñaut Izagirre, Pablo Domínguez Aguilar, Javier Bandrés, Francisco Rojas Heredia, Oriol Monserrat, and Juan Ignacio López Moreno

The Pyrenees range is the most southern European region with active glaciers and rock glaciers. In the current climate change context, their depth, extent and viability are rapidly declining. Even though they are usually located in high-elevation and remote areas, their dynamics can affect human settlements and activities. Mapping and monitoring these ice bodies will provide more information about their past, present and future evolution.

Remote sensing data provides extensive information, especially in rough mountainous areas and inaccessible or distant regions. Differential and Multitemporal interferometry (DInSAR and MT-InSAR) has been extensively proven to be a valuable tool to detect ground deformations, but also works to provide insightful results over glacial and periglacial environments. Since many authors have found SAR data useful in this context, there is a scarcity of works that exploit the high spatial and temporal resolution of X-band dense constellations such as COSMO-SkyMed. On the other hand, this kind of ice bodies are usually located over low satellite-visibility areas (related to shadow and layover effects), increasing the importance of alternative information, such as that provided by in-situ (GNSS) or near-remote sensing (UAV).

This work compares coverture and displacement results from Sentinel-1 C-band (both DInSAR and MT-InSAR) and COSMO-SkyMed X-band data. MT-InSAR results from EGMS revealed low coverage due to geometrical and snow-cover issues, while DInSAR results from both constellations provide better coverage results. UAV flights over the glacier allowed perfect coverage and high spatial resolution, but lacked in temporal resolution. Lastly, a GNSS measurement grid was redeployed over the glacier and will provide displacement data for future campaigns and for comparison with previous campaigns in the 90s. Combining data from UAV flights, three-dimensional displacement is estimated and compared with InSAR results, after projection in the Line of Sight (LOS), with the InSAR displacements. This work is part of JDC2023-052719-I, financed by MCIU/AEI/10.13039/501100011033 y and FSE+.

How to cite: Ezquerro, P., Revuelto, J., López-Vinielles, J., Izagirre, E., Domínguez Aguilar, P., Bandrés, J., Rojas Heredia, F., Monserrat, O., and López Moreno, J. I.: Monitoring Argualas rock glacier dynamics combining InSAR, GNSS and UAV data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22830, https://doi.org/10.5194/egusphere-egu26-22830, 2026.

EGU26-461 | ECS | Orals | CR1.4

Early Alpine glaciations at ca. 2 Ma revealed by 26Al–10Be burial dating of endokarst sediments in the western–central European Alps 

Vivien Mai Yung Sen, Pierre Valla, Stéphane Jaillet, Xavier Robert, Yann Rolland, Miguel Borreguero, Julien Carcaillet, Edwige Pons-Branchu, Christian Crouzet, and Olivier Bruguier

The onset and potentially time-transgressive latitudinal development of Northern Hemisphere glaciations during the Plio-Quaternary represents a key component of global late Cenozoic climate dynamics. The timing of the earliest Alpine glaciations has been debated since the pioneering work of A. Penck and E. Brückner at the beginning of the 20th century. Over the past three decades, cosmogenic nuclide burial dating has provided absolute ages on glacial and fluvioglacial sedimentary deposits in the Alpine forelands, progressively refining the chronology of early glaciations as methodological advances have emerged and as the number of analyzed samples has increased. Recent syntheses from the northern Alpine foreland (Deckenschotter) and the Ivrea amphitheater indicate that piedmont glacier lobes developed between 1.2 and 0.8 Ma, suggesting that the first extensive Alpine-wide glaciations occurred during the Mid-Pleistocene Transition. However, reconstructions based solely on surface deposits are strongly affected by preservation biases, as repeated glaciations may have eroded older sedimentary archives. As a result, Early Pleistocene surface records may have been largely removed by subsequent, more extensive glaciations.

Karst systems provide an alternative archive for early glaciations. During glacial periods, glaciers in contact with karst conduits inject detrital material (allochthonous or autochthonous) into subsurface voids, where sediments can be preserved for several million years. These buried deposits can be dated using in situ cosmogenic nuclides such as 26Al–10Be in quartz. Prior to this study, very few geochronological and sedimentological data existed for such ancient glacio-karst deposits (i.e. Early Pleistocene). New 26Al–10Be burial ages obtained from 20 detrital endokarst sediment samples (sands and pebbles) in the western to central Alps (Vercors, Chartreuse, Haut-Giffre and Bernese Alps), together with a synthesis of existing dating in the central Alps, allow the first spatio-temporal reconstruction of glacial sediment injections into the Alpine karst. Consistent with surface records, the burial ages reveal major glacial sediment injections into the karst around 0.8 Ma, at the end of the Mid-Pleistocene Transition. However, the data also point to a much earlier phase of widespread injections around 2 Ma. These early injections occurred both in high-elevation (>2500 m) headwater karst systems and in peripheral karst networks bordering the major Alpine valleys along the mountain front, demonstrating that widespread early glaciations affected the entire Alpine chain around 2 Ma. Because Alpine valleys were less deeply incised during the Early Pleistocene, glacier geometries differed significantly from those of Middle and Late Pleistocene glaciations, with thinner and potentially less extensive ice bodies. These earliest Alpine glaciations are contemporaneous with major advances of the Eurasian and North American ice sheets, consistent with extensive Northern Hemisphere glaciations at that time, predating the intensification of glaciations initiated at the Mid-Pleistocene Transition. Ultimately, this study highlights the potential of mountain karst systems as long-term archives for reconstructing Quaternary climate transitions.

How to cite: Mai Yung Sen, V., Valla, P., Jaillet, S., Robert, X., Rolland, Y., Borreguero, M., Carcaillet, J., Pons-Branchu, E., Crouzet, C., and Bruguier, O.: Early Alpine glaciations at ca. 2 Ma revealed by 26Al–10Be burial dating of endokarst sediments in the western–central European Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-461, https://doi.org/10.5194/egusphere-egu26-461, 2026.

EGU26-822 | Orals | CR1.4

Using digital mapping and cosmogenic 10Be to assess glacial landscape modification in west-central Keewatin, Arctic Canada  

Clara Crowell, Sam Kelley, Etienne Brouard, Janet Campbell, and John Gosse

The west-central Keewatin region of northern Canada preserves a rich record of former ice sheets and their impact on the landscape. The diverse assemblage of glacial landforms in the region reflects spatial variations in glacial modification driven by changes in basal thermal regime, subglacial hydrology, and ice-flow dynamics, all of which are key to reconstructing the history and behaviour of palaeo-ice sheets. Resolving how these landforms relate to changes in basal regime and glacial modification requires integrated datasets such as geomorphological mapping and to provide the robust reconstructions needed for climate and ice-sheet models.

Our work aims to provide both a qualitative and quantitative assessment of glacial landscape modification in the west-central Keewatin region of the Northwest Territories and mainland Nunavut using two independent proxies: geomorphic mapping and cosmogenic nuclide concentrations. We used the ArcticDEM and Landsat 8 imagery to remotely map This new inventory of landforms, integrated with existing mapping, provides a qualitative assessment of glacial landsystems and landscape modification across the Keewatin region. As a quantitative proxy for glacial modification from the last glacial period(s), we collected 10 bedrock and 7 boulder samples for cosmogenic 10Be measurement along a north-south transect east of Dubawnt Lake, Nunavut. The sample transect was informed by glacial geomorphic mapping and was selected to test field-based predictions of the degree of landscape modification from the previous glaciation(s). The northern portion of the transect contains high concentrations of streamlined landforms associated with the onset zone of the Dubawnt Ice stream, inferred to be a region of high glacial modification. In contrast, the southern end of the transect contains lower concentrations of streamlined features, flow sets with contrasting orientations, and cross-cutting striations, suggesting a higher degree of landscape preservation during the last glaciation(s). Preliminary 10Be results broadly confirm our initial assessment of glacial modification along our transect, revealing slightly higher concentrations of 10Be in the south (less modification) and decreasing 10Be concentrations towards the north (more modification). Both bedrock and boulder samples follow this trend, however, our results show that in both low- and high-modification landsystems, some samples retain significant nuclide inheritance, including some boulders which suggests transport from a less modified landscape. Combining qualitative and quantitative approaches to evaluate glacial modification associated with specific landform assemblages informs our understanding of the basal thermal conditions of palaeo-ice sheets, the distribution of which informs our understanding of ice sheet evolution through space and time. Furthermore, the identification of streamlined features into palaeo-flow sets supports potential mineral exploration by helping to determine glacial transport directions and dispersal patterns. However, our results show the concentrations of cosmogenic nuclides vary within individual landsystems, suggesting that glacial modification varied through time and can be influenced by multiple factors (e.g., subglacial thermal conditions, topography, glacio-isostatic adjustment, lake development) that remain to be quantified.  

How to cite: Crowell, C., Kelley, S., Brouard, E., Campbell, J., and Gosse, J.: Using digital mapping and cosmogenic 10Be to assess glacial landscape modification in west-central Keewatin, Arctic Canada , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-822, https://doi.org/10.5194/egusphere-egu26-822, 2026.

EGU26-1360 | ECS | Orals | CR1.4

Cosmogenic chlorine-36 constraints on Holocene glacier change in Iceland 

Aylin de Campo, Shaun Eaves, Kevin Norton, Klaus Wilcken, Réka-Hajnalka Fülöp, Krista Simon, Carla Silvia, Timothy Lane, and Margaret Jackson

Understanding temperature variability during the Holocene is critical for constraining baselines of natural climate variability. Temperate mountain glacier extent is limited most significantly by summer air temperature, thus geological records of past glacier length changes represent a useful proxy for this climatic variable. Iceland’s maritime glaciers with their high sensitivity to temperature and precipitation changes serve as robust indicators of climate variability in the North Atlantic region. Previous reconstructions of Iceland’s Holocene glacier and climate history have relied primarily on marine sediment cores, terrestrial geomorphological evidence, and glaciological modelling. These proxies highlight a correlation between glacier fluctuations and regional climate variability and suggest notable glacier retreats during early and mid-Holocene warm periods.

Here, we present cosmogenic chlorine-36 measurements from four outlet glaciers of the Vatnajöküll ice cap in Iceland that test and further constrain the occurrence of past glacier minima during the Holocene. Unlike the more commonly used method of cosmogenic surface exposure dating of moraines, which constrains the timing of past glacier advances, our application targets the remnant cosmogenic signals of prehistoric exposure events preserved in freshly exposed proglacial surfaces. Our data thus tests for the occurrence and constrains the duration of past glacier retreat events and, thereby, warmer times during the Holocene. Our results support the hypothesis that Icelandic glaciers were smaller than present for several millennia during the Holocene and when combined with existing datasets of Icelandic climate, our new results allow us to reconstruct both glacier advance and retreat through the Holocene.

How to cite: de Campo, A., Eaves, S., Norton, K., Wilcken, K., Fülöp, R.-H., Simon, K., Silvia, C., Lane, T., and Jackson, M.: Cosmogenic chlorine-36 constraints on Holocene glacier change in Iceland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1360, https://doi.org/10.5194/egusphere-egu26-1360, 2026.

EGU26-2751 | Posters on site | CR1.4

Symmetrical till-cored drumlins highlight where past ice sheets flowed faster 

John K. Hillier, Mike Smith, Tom Dowling, Matteo Spagnolo, John Maclachlan, and Carlos Martin

For over 100 years, from school textbook to research, glacially sculpted landforms called drumlins have been considered asymmetrical, tear-drop shaped. Recent work has securely demonstrated that, in the absence of bedrock, this asymmetry is measurable but tiny – non-existent to visual inspection.  High-resolution DEMs and a novel application of statistics to flow-sets demonstrate that a well-studied a Swedish site exhibits a transition from asymmetrical bedrock-cored drumlins to symmetrical till-cored ones within just a few 10s of m of till. We believe that this is the first direct observational constraint upon the thickness of till required to effectively decouple flowing ice from rough bedrock topography.  Understanding where till lubrication has the potential to speed up ice flow has large implications for modelling current ice sheets and Antarctic deglaciation, so we are hoping for ideas of how to best assess this last part.

How to cite: Hillier, J. K., Smith, M., Dowling, T., Spagnolo, M., Maclachlan, J., and Martin, C.: Symmetrical till-cored drumlins highlight where past ice sheets flowed faster, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2751, https://doi.org/10.5194/egusphere-egu26-2751, 2026.

EGU26-3417 | Orals | CR1.4

New evidence for Greenland ice sheet expansion beyond its present shelf break during the Mid-Pleistocene Transition   

Jochen Knies, Henry Patton, Peter-Lasse Giertzuch, and Stijn De Schepper and the i2B Arctic Ocean Expedition 2025 Science Party

The possibility of a continuous, kilometre-thick Arctic Ocean ice shelf in the geological past has long intrigued scientists. Yet, fundamental questions surrounding the architecture, timing, and oceanic and climatic consequences of such an ice shelf remain unresolved. A pan-Arctic glaciation model has been inferred primarily from glacial landforms identified on seafloor bathymetric highs and continental shelves, as well as from geochemical proxies found in marine sediment cores.

Subsequent chronological analyses of sediment cores from these eroded regions have suggested that this pan-Arctic Ocean ice shelf developed during Marine Isotope Stage (MIS) 6, approximately 140,000 to 160,000 years ago. In contrast, more recent evidence from the eastern Fram Strait suggests the persistence of marginal sea-ice conditions and recurrent phytoplankton spring blooms across several glacial-interglacial cycles over the last 750,000 years. Nevertheless, an exception appears to occur during MIS 16, a glacial interval between ~670,000 and 620,000 years ago that remains relatively understudied in the Arctic Ocean. During this period, biomarkers indicative of sea ice and primary productivity, and planktic foraminifera are either absent or occur in extremely low concentrations in sediment cores from both the Arctic-Atlantic Gateway and the Nordic Seas. Although the full spatial extent of glacial ice during MIS 16 remains uncertain, it is thought to have rivalled that of the Last Glacial Maximum (LGM) in terms of ice volume. In this study, we present new geomorphological evidence supported by sediment core chronologies for significant Greenland ice sheet expansion during the end of the Mid Pleistocene Transitoin (MPT). The discovery of record-deep ploughmarks, in combination with a grounding zone wedge (GZW) at approximately 800 meters water depth on the Morris Jesup Rise, northeast Greenland, suggests that the Greenland/Innuitian Ice Sheet grew sufficiently to form an ice shelf extending into the central Arctic Ocean – implying an "Antarctification" of Greenland during this extreme glacial phase.

 

How to cite: Knies, J., Patton, H., Giertzuch, P.-L., and De Schepper, S. and the i2B Arctic Ocean Expedition 2025 Science Party: New evidence for Greenland ice sheet expansion beyond its present shelf break during the Mid-Pleistocene Transition  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3417, https://doi.org/10.5194/egusphere-egu26-3417, 2026.

EGU26-4936 | ECS | Posters on site | CR1.4

Chasing pavements: New insights from Late Palaeozoic glacial outcrops in South Africa 

Ricarda Wohlschlägl, Paulina Mejías Osorio, Marie Busfield, Peter Haberer, Albertus Smith, and Daniel Le Heron

During the Late Palaeozoic Ice Age (LPIA; ~360–260 Ma), southern Africa formed part of Gondwana and experienced repeated episodes of continental glaciation. These glacial events left an extensive sedimentological and geomorphological record. In several regions, modern topography partially reflects this inherited glacial relief, providing rare insights into pre-Quaternary ice-sheet dynamics, basal processes, and ice–substrate interactions. Despite their scientific importance, many LPIA glacial pavements in southern Africa remain poorly documented and understudied. Numerous key outcrops are increasingly threatened by natural erosion, flooding, agricultural practices, and industrial development. In addition, access is often restricted because many pavements occur on private farmland or in remote areas, limiting systematic field investigation. To date, most known glacial pavements have not been digitally mapped or analysed at high spatial resolution. 

Here we apply integrated aerial and close-range photogrammetry, combined with detailed sedimentological analysis, to document seven representative Late Palaeozoic glacial outcrops in the Northern Cape Region in South Africa. High-resolution digital outcrop models are complemented by field-based sedimentological observations. Together, these approaches provide a robust framework for interpreting glacial dynamics and depositional environments. The resulting digital and sedimentological datasets form a reproducible archive that supports quantitative analysis, virtual access, and long-term preservation of vulnerable geological heritage sites. Our results demonstrate the potential of combining digital documentation with in-depth sedimentological analysis to advance the study of ancient glacial landscapes and to preserve critical pre-Quaternary cryospheric records for future research.

How to cite: Wohlschlägl, R., Mejías Osorio, P., Busfield, M., Haberer, P., Smith, A., and Le Heron, D.: Chasing pavements: New insights from Late Palaeozoic glacial outcrops in South Africa, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4936, https://doi.org/10.5194/egusphere-egu26-4936, 2026.

EGU26-6359 | Posters on site | CR1.4

Constraining fjord formation and isostatic uplift in Arctic Canada and Northeast Greenland using Pliocene-early Pleistocene sediment deposits 

Vivi Kathrine Pedersen, Caroline Brand, Nicolaj Krog Larsen, and Jonas Folmer Damsgård

In Arctic Canada and Northeast Greenland, previous studies have found several high-elevation occurrences of marine and/or fluvial sediments of Pliocene-early Pleistocene age. In Arctic Canada, the deposits include the marine strata of the Hvitland beds on Ellesmere Island (up to ~130 m a.s.l.; Fyles et al., 1998), the marine deposits on Meighen Island (up to ~100 m a.s.l.; Fyles et al., 1991), as well as several sites with fluvial deposits, including the unconsolidated braided river deposits found on Banks Island (up to ~130 m a.s.l.; e.g., Fyles et al., 1994), Prince Patrick Island (up to ~200 m a.s.l.; Fyles, 1990), and on the high terraces of Ellesmere Island (up to ~600 m a.s.l.; Fyles, 1989) – all assumed to have be deposited prior to the carving of the deep fjord systems seen in the regions today. In Northeast Greenland, the sediment deposits include the marine Kap København (up to ~230 m; Funder et al., 1984) and Lodin Elv Formations (up to 62 m a.s.l.; Feyling-Hansen et al., 1983), assumed to have been deposited ca. 2-2.5 Ma. Previous work has studied these deposits in detail to constrain their fauna and age, their stratigraphic relationships, as well as their implications for past climates in the Arctic. However, particularly the current high elevation of the marine deposits can also put time constraints on surface uplift in these regions (e.g., Pedersen et al., 2019). Here we explore these constraints in the context of erosion driven flexural isostatic uplift associated with glacial erosion and fjord formation, allowing us to constrain the incision of the fjord systems in time, with the potential to also constrain the timing and rates of glacial erosion.

Feyling-Hanssen, R.W., Funder, S., Petersen, K.S., 1983, The Lodin Elv Formation: A Plio-Pleistocene occurrence in Greenland. Bulletin of the Geological Society of Denmark 31, 81-106.

Funder, S., Bennike, O., Mogensen, G.S., Noe-Nygaard, B., Pedersen, S.A.S., Petersen, K.S., 1984. The Kap København Formation, a late Cainozoic sedimentary sequence in North Greenland. Grønlands Geologiske Undersøgelse, 120, 9–18.

Fyles, J.G., 1989: High terrace sediments probably of Neogene age, west-central Ellesmere Island, Northwest Territories; in Current Research, Part D; Geological Survey of Canada, Paper 89-1 D, p. 101-104.

Fyles, J.G., 1990. Beaufort Formation (Late Tertiary) as seen from Prince Patrick Island, Arctic Canada. Arctic 43, 393-403.

Fyles, J.G., Marincovich, L., Jr., Matthews, J.V., Jr., Barendregt, R., 1991. Unique mollusc find in the Beaufort Formation (Pliocene) on Meighen Island, Arctic Canada; in Current Research, Part B; Geological Survey of Canada, Paper 91-1 B, 105-112.

Fyles, J.G., Hills, L.V., Matthews, J.V., Barendregt, R., Baker, J., Irving, E., Jetté, H., 1994. Ballast Brook and Beaufort Formations (late Tertiary) on Northern Banks Island, Arctic Canada. Quaternary International 22–23, 141-171.

Pedersen, V.K., Larsen, N.K., Egholm, D.L., 2019. The timing of fjord formation and early glaciations in North and Northeast Greenland. Geol­ogy 47, 682–686.

How to cite: Pedersen, V. K., Brand, C., Krog Larsen, N., and Folmer Damsgård, J.: Constraining fjord formation and isostatic uplift in Arctic Canada and Northeast Greenland using Pliocene-early Pleistocene sediment deposits, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6359, https://doi.org/10.5194/egusphere-egu26-6359, 2026.

EGU26-9053 | ECS | Posters on site | CR1.4

SIBERICE v1: a database of Quaternary glacial reconstructions, glacial geomorphology, and chronometric data in Siberia 

Benjamin Boyes, Iestyn Barr, Rachel Oien, Izabela Szuman, Monica Winsborrow, and Martin Margold

The Quaternary glacial history of Siberia is uncertain, with several competing reconstructions existing in the published literature. This uncertainty is driven by seemingly incomplete and inconsistent records of glacial geomorphology and a patchy record of chronometric data. To address this, we have compiled previously published glacial geomorphological maps and chronometric data to establish what empirical data for former glaciations exist across Siberia. We also use these data to test the currently published glacial reconstructions to determine which, if any, reconstruction can be best underpinned by current empirical evidence. In turn, we will attempt to reconcile the competing reconstructions into coherent glaciation scenarios for the Quaternary stadials or highlight where palaeo-glaciological research is needed.

Here, we present version-1 of the SIBERICE database, a compilation of all previously published glacial geomorphology, chronometric data, and glacial reconstructions published up to 1 January 2026. The SIBERICE database is a Geographic Information System (GIS) database that make data readily accessible, including information published in often overlooked Russian-language journal articles.

How to cite: Boyes, B., Barr, I., Oien, R., Szuman, I., Winsborrow, M., and Margold, M.: SIBERICE v1: a database of Quaternary glacial reconstructions, glacial geomorphology, and chronometric data in Siberia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9053, https://doi.org/10.5194/egusphere-egu26-9053, 2026.

EGU26-9543 | Orals | CR1.4

Soft-bed distributed subglacial sedimentology 

Jane Hart and Kirk Martinez

The nature of the subglacial environment is a key part of glacier dynamics. Studies from modern glaciers have revealed there is a continuum in subglacial fluvial behaviour associated with a soft-bed, from channelised to distributed. How is this continuum preserved within the sedimentary record and what is the relationship between fluvioglacial sediments and flutes?  Classically eskers are associated with channelized drainage, whilst the sedimentary remains of ‘canals’, ‘subglacial meltwater corridors’ and murtoos may reflect the distributed system. Stratified lenses within till are common and have been given numerous interpretations, either reflecting preglacial sediments that have been incorporated into the till by deformation, or penecontemporaneous sedimentation with the till. We use data from instrumented modern glaciers and Quaternary sections to illustrate the nature and rate of subglacial behaviour associated with soft-bedded glaciers.

How to cite: Hart, J. and Martinez, K.: Soft-bed distributed subglacial sedimentology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9543, https://doi.org/10.5194/egusphere-egu26-9543, 2026.

EGU26-10117 | Orals | CR1.4

Reconstructing Plio-Quaternary fluctuations of the East Antarctic Ice Sheet in Terre Adélie inferred from cosmogenic nuclides (10Be-26Al) in glacially-polished bedrock, morainic boulders and nunataks  

Yann Rolland, Marcelline Péan, Pierre Valla, Guillaume Duclaux, Régis Braucher, Vincent Jomelli, Vincent Favier, Irene Schimmelpfennig, Xavier Crosta, Johan Etourneau, and Margot Louis

The East Antarctic Ice Sheet (EAIS) contribution for future global sea level rise and climate change is source of uncertainty, and it appears essential to reconstruct its past fluctuations. Previous works reveal geomorphic and chronological evidence that the ice sheet extended to the continental shelf break during LGM (Last Glacial Maximum; ~20 ka). However, still little is known about its response to the major climate and oceanic transitions following the LGM. In this study, we reconstruct (1) a chronology of ice-sheet fluctuations, (2) ice-sheet past erosion efficiency and (3) ice-sheet thinning during the late-Pleistocene to Holocene time-period, in Terre Adélie (East Antarctica). Newly obtained exposure ages for coupled 10Be-26Al support a scenario of glacial fluctuations at global, regional and local scales. Inland nunataks reveal some long-term exposure with apparent exposure ages ~150 ka, while coastal areas record a past ice-sheet thinning after ~20 ka. Ages measured on erratic boulders of Archipel Pointe Géologie record the final episode of a regional deglaciation around ~15 ka. Slightly inland, in Lacroix sector, erratic boulders record a more recent local ice-sheet oscillations around ~1.5 ka. In contrast, exposure ages obtained on glacially-polished bedrock are characterised by spatially-variable inheritance, suggesting that past ice sheet retreat history is characterised by variations in erosion efficiency. Finally, our results also suggest some potential previous geomorphological inheritance from the hot Pliocene phase.

How to cite: Rolland, Y., Péan, M., Valla, P., Duclaux, G., Braucher, R., Jomelli, V., Favier, V., Schimmelpfennig, I., Crosta, X., Etourneau, J., and Louis, M.: Reconstructing Plio-Quaternary fluctuations of the East Antarctic Ice Sheet in Terre Adélie inferred from cosmogenic nuclides (10Be-26Al) in glacially-polished bedrock, morainic boulders and nunataks , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10117, https://doi.org/10.5194/egusphere-egu26-10117, 2026.

EGU26-10565 | ECS | Posters on site | CR1.4

Vernagtferner flute field findings, Austrian Alps 

Paulina Mejías Osorio, Ricarda Wohlschlägl, Sara Karbacher, Thomas Vandyk, Bethan J. Davies, Bernhard Grasemann, and Daniel P. Le Heron

Glacial forefields host abundant information regarding the sedimentary processes associated with glacier dynamics. Transport pathways and sediment deposition can be characterized by investigating the landforms and sediments found in these areas. One such area is the Vernagtferner forefield in the Austrian Alps, which contrasts with other surrounding glaciers due to the presence of a large surface covered by flutes. These flutes can reach up to 250 m in length and have been continuously exposed over the past decades as the glacier recedes, but have not been researched recently. Since this glacier has been regularly studied (with records from as early as 1601) and it has been linked to surging episodes in the past, there are plenty of questions to be answered related to its current behavior. Here we present the results of sedimentological observations, as well as geomorphological mapping and statistics based on fieldwork, historical, and uncrewed aerial vehicle imagery. We highlight aspects of the glacial forefield and the contrast between what can be seen in 2023-2024 and snapshots from the past 50 years. In a changing climate, understanding how rapid glacial recession affects the deposition of sediments and the parameters that govern them will be useful in deciphering glacial dynamics and contrasting them with the paleorecord. 

How to cite: Mejías Osorio, P., Wohlschlägl, R., Karbacher, S., Vandyk, T., Davies, B. J., Grasemann, B., and Le Heron, D. P.: Vernagtferner flute field findings, Austrian Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10565, https://doi.org/10.5194/egusphere-egu26-10565, 2026.

EGU26-11727 | ECS | Orals | CR1.4

Modelling the evolution of Dronning Maud Land, Antarctica across the last interglacial-glacial cycle – insights from isochrone modelling. 

Vjeran Višnjević, Julien Bodart, Antoine Hermant, Emma Spezia, Christian Wirths, and Johannes Sutter

Reconstructions of Antarctica's past ice-sheet evolution remain poorly constrained due to sparse, spatially discontinuous proxies, limiting accurate projections of its future sea-level contribution. Here we present a novel isochronally-constrained reconstruction of Dronning Maud Land (DML), East Antarctica spanning the last interglacial-glacial cycle (~130 kyr), integrating extensive radar-derived internal reflection horizons (IRHs) with PISM ice-sheet simulations.

IRHs preserve continuous records of past accumulation, flow, and basal conditions, providing unprecedented spatiotemporal constraints for model validation. Our ensemble simulations indicate that DML’s sea-level potential change between interglacial and glacial states is comparable to, and likely larger than, the contribution of all modern mountain glaciers, and show that variations in geothermal flux alone can substantially alter sea-level projections. These results provide physical modelling context of East Antarctica's ice history, reveal DML's role in Last Interglacial sea-level rise, and highlight persistent parameterization uncertainties limiting future projections.

How to cite: Višnjević, V., Bodart, J., Hermant, A., Spezia, E., Wirths, C., and Sutter, J.: Modelling the evolution of Dronning Maud Land, Antarctica across the last interglacial-glacial cycle – insights from isochrone modelling., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11727, https://doi.org/10.5194/egusphere-egu26-11727, 2026.

EGU26-11797 | ECS | Posters on site | CR1.4

Constraining Early and Middle Pleistocene Laurentide Ice Sheet advances with 10Be-26Al burial dating 

Ruben Bertels, Kaleb Wagner, Lotta Ylä-Mella, Benjamin J. Stoker, John D. Jansen, and Martin Margold

Throughout the Quaternary, cyclical variations in global ice volume are recorded by benthic marine δ18O fluctuations. This signal is dominated by the waxing and waning of Northern Hemisphere ice sheets, particularly the Laurentide Ice Sheet (LIS) in North America, which builds periodically into the largest of all ice sheets on Earth. At such times, the LIS advanced southward into the American Midwest where glacial deposits emplaced prior to Marine Isotope Stage (MIS) 6 are known from just a handful of securely-dated sites. Consequently, current understandings of LIS extent and volume through time are incomplete and poorly constrained.

Here, we focus on tills bearing putative pre-MIS 6 depositional ages along the southern and southwestern margins of the LIS. We combine single-grain sedimentary provenance analyses with cosmogenic 10Be-26Al burial dating in an aim to better resolve till chronology and provenance, using P-PINI and CosmoChron numerical models to calculate burial ages.

Building on existing magneto-, tephro-, and lithostratigraphic correlations, our new burial ages will significantly improve knowledge of the timing and extent of the LIS and its sediment source areas feeding different ice sheet sectors along the southern and southwestern margins. Our findings will improve reconstructions of LIS configurations through time, and yield new insights into Early–Middle Pleistocene global ice volume variability linked directly to the terrestrial record.

How to cite: Bertels, R., Wagner, K., Ylä-Mella, L., Stoker, B. J., Jansen, J. D., and Margold, M.: Constraining Early and Middle Pleistocene Laurentide Ice Sheet advances with 10Be-26Al burial dating, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11797, https://doi.org/10.5194/egusphere-egu26-11797, 2026.

EGU26-12234 | ECS | Orals | CR1.4

From source to sink: Quantifying Quaternary erosion from offshore deposits associated with the Greenland Ice Sheet 

Caroline Brand, Judith Elger, Katrine Juul Andresen, Thomas Mejer Hansen, Victor Sixto Poulsen, Lara F. Pérez, Matthew Fox, Christoph Böttner, Paul Knutz, Jonas Folmer Damsgård, and Vivi Kathrine Pedersen

Glacially derived, marine sediments preserve a record of the timing, extent, and dynamics of shelf glaciation. In addition, these deposits can provide constraints on glacial erosion rates and offer insights into landscape evolution. However, in Greenland, the total offshore volume of glacially derived sediments remains poorly constrained due to an uneven distribution of offshore seismic surveys and a lack of dating constraints. To address this, we present a first quantification of Quaternary glacial sediment thicknesses around Greenland, combining interpretations of available marine seismic data with age constraints where scientific boreholes are available and a neural network approach. We train the neural network using the seismic-derived thicknesses, along with several parameters related to glacial and geomorphological features. This approach allows us to predict Quaternary sediment thicknesses in regions with sparse data coverage, thereby constraining the total volumes of deposition. Our estimates reveal regional variations in glacial deposition volumes and sediment thicknesses around Greenland. On the southern and parts of the northern Greenlandic continental slope, Quaternary sediments are thin, whereas in west and east Greenland, larger sediment deposits have led to a greater shelf progradation throughout the Quaternary. These patterns demonstrate a diverse influence of (paleo-)climatic, oceanographic, and orographic processes on glacial dynamics and the source-to-sink sediment transport. Finally, we compare our estimates of Quaternary offshore deposition with estimates of onshore glacial erosion inferred from paleo-topographic reconstructions and erosion potentials of the present ice sheet, based on ice sliding velocities. This provides insights into the temporal and spatial variability of erosion around Greenland, advancing our understanding of the long-term landscape evolution in glaciated regions.

How to cite: Brand, C., Elger, J., Andresen, K. J., Hansen, T. M., Poulsen, V. S., Pérez, L. F., Fox, M., Böttner, C., Knutz, P., Damsgård, J. F., and Pedersen, V. K.: From source to sink: Quantifying Quaternary erosion from offshore deposits associated with the Greenland Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12234, https://doi.org/10.5194/egusphere-egu26-12234, 2026.

EGU26-12657 | Posters on site | CR1.4

The formation of flute fields in glacial environments 

Daniel Le Heron, Marie Busfield, Paulina Mejías Osorio, Bertus Smith, Saeed Tofaif, and Ricarda Wohlschlägl

Understanding the processes at glacier beds is crucial as they regulate ice flow, basal sediment dynamics, and meltwater routing, which collectively control glacier stability and response to climate change. Flute fields are a vital archive of subglacial processes, widespread in both terrestrial and marine glacial environments, whereby sediments are fashioned subglacially into lineations at different scales. The assemblages are highly variable in both environments, yet models to explain this are outstanding, and aspects of preservational bias are rarely entertained. Integrating observations from modern Alpine forefields (Austria) with exceptionally preserved Late Ordovician and Late Paleozoic examples in Africa and Arabia, we interrogate terrestrial and glaciomarine flute fields. Flutes, megaflutes, and diamictons occur in both settings, but architecture is strongly context-dependent. Terrestrial flutes degrade rapidly under surface meltwater and rainfall, whereas marine flute fields are commonly preserved beneath fine-grained shales, recording stacked lobate sediments with superimposed mega-scale glacial lineations, metre-scale flutes, and centimetre-scale soft-sediment striae. Oversteepened subaqueous flutes collapse laterally, forming fan-shaped deposits, and lateral margins exhibit scalloped surfaces that record focused subglacial meltwater discharge. We propose a conceptual model in which metre- and centimetre-scale lobes act as miniature grounding zone wedges, forming through simultaneous deposition and shearing beneath tidewater glaciers. This framework reveals how subglacial processes are recorded in preserved landforms and demonstrates that integrating modern and ancient records is essential to understanding glacier–bed interactions.

How to cite: Le Heron, D., Busfield, M., Mejías Osorio, P., Smith, B., Tofaif, S., and Wohlschlägl, R.: The formation of flute fields in glacial environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12657, https://doi.org/10.5194/egusphere-egu26-12657, 2026.

EGU26-12949 | ECS | Posters on site | CR1.4

Glacial-interglacial cycles in the Western Alps (Middle Durance Valley, France): sedimentary evolution and responses of continental surfaces 

Virgile Dervis, Alexis Nutz, Magali Rizza, Régis Braucher, Pierre Dietrich, and Hélène Tissoux

The existence of glacial cycles in the Alps was proposed as early as the first half of the 19th century following the observation of numerous direct traces left by glaciers in lower parts of alpine valleys. However, the influence of glacial-interglacial cycles on sediment transfer from the internal source zone to the peripheral mountain range is only now being re-investigated in the context of the recent “Source to sink” approach.

The study, part of the DYMODU project (2023–2026), a collaboration between the CNRS and the RGF focuses on new geological, geomorphological and geochronological investigations undergone in the Laragne-Montéglin depression and along the Middle Durance (western Alps, France). The DYMODU project aims at deciphering the role of glacial-interglacial cycles in both the landscape organization of alpine valleys and the evolution of routing systems during the Quaternary. The sediment pile shows a characteristic sedimentary motif repeated four times, indicating a succession of four aggradation-incision cycles. The sedimentary motif records a period of aggradation during which a several tens of metres thick conglomerate fills one or more palaeo-valleys, affecting the underlying units. This conglomerate is topped by glaciogenic deposits (ground till, morainic vallum), then incised by one or more palaeo-valleys affecting the entire sedimentary series, often down to the underlying sediments before the onset of the aggradation phase of the next cycle begins, and fills these palaeo-valleys.

To confirm the integration of these cycles into the Quaternary evolution of the area, preliminary dating was carried out on various sedimentary morphostructures using Optically Stimulated Luminescence dating (OSL), Electron Spin Resonance dating (ESR) and Cosmogenic Nuclides (CN).

In this contribution, we will present the sedimentary pattern of a typical sequence. We will attempt to deconvolute the signals of the general Alpine uplift, the lithospheric flexure due to glaciation, and the glacio-isostatic rebound during deglaciation. This will enable us to discuss the interdependencies between climate and tectonics for valley glacier systems and the forcings that influenced sediment routing during the Upper Pleistocene in the Alps.

How to cite: Dervis, V., Nutz, A., Rizza, M., Braucher, R., Dietrich, P., and Tissoux, H.: Glacial-interglacial cycles in the Western Alps (Middle Durance Valley, France): sedimentary evolution and responses of continental surfaces, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12949, https://doi.org/10.5194/egusphere-egu26-12949, 2026.

EGU26-14137 | ECS | Posters on site | CR1.4

Deglaciation of the Ardencaple Fjord and adjacent shelf environment, Northeast Greenland 

Mads Ramsgaard Stoltenberg, Karoline Kristensen, Christoph Böttner, Adrián López-Quirós, Joanna Davies, Juliette Girard, Henrieka Detlef, Guillaume St‐Onge, Christof Pearce, and Marit-Solveig Seidenkrantz

In this study, we integrate marine geophysical datasets and analyses of four marine sediment cores to reconstruct the deglaciation and paleoenvironmental development of the Ardencaple Fjord and the adjacent cross-shelf trough in Northeast Greenland. Although recent studies have presented isochron-based reconstructions of the circum-Greenland ice margin since the last deglaciation, crucial knowledge gaps regarding the timing and dynamics of ice retreat still exist, particularly in offshore Northeast Greenland, where former glaciated trough systems hosted fast-flowing ice.

Our preliminary results indicate fast retreat dynamics of the ice based on observations of glacial lineation morphologies on the seabed, while sedimentological data enable spatiotemporal reconstructions of grounding line positions and floating ice margins. A preliminary chronological framework constraining the ice retreat across the core sites is based on radiocarbon dates, supplemented by paleomagnetic secular variation records. Our reconstruction further allows us to assess benthic ecosystem responses to deglaciation, contributing to the current evaluation of benthic foraminifera as a proxy for identifying stages of deglaciation in marine sediments around Greenland.

How to cite: Ramsgaard Stoltenberg, M., Kristensen, K., Böttner, C., López-Quirós, A., Davies, J., Girard, J., Detlef, H., St‐Onge, G., Pearce, C., and Seidenkrantz, M.-S.: Deglaciation of the Ardencaple Fjord and adjacent shelf environment, Northeast Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14137, https://doi.org/10.5194/egusphere-egu26-14137, 2026.

EGU26-14254 | Posters on site | CR1.4

Deglaciation of the ancestral Kangerlussuaq Glacier from the continental shelf offshore of SE Greenland following the LGM 

Colm O'Cofaigh, Matthew Hunt, Jeremy Lloyd, Kelly Hogan, Camilla Snowman Andresen, Robert Larter, and David Roberts

Marine geophysical data and sediment cores were collected from the continental shelf and slope offshore of SE Greenland during cruise SD041 of the UK research vessel the RRS Sir David Attenborough in 2024. The cruise collected a range of geological, geophysical, oceanographic and biological data. The cruise was part of the ‘Kang-Glac’ project, the aim of which is to investigate the response of the Greenland Ice Sheet to ocean warming during the last 11,700 years. Marine geophysical data and radiocarbon-dated sediment cores provide a clear record of an extensive Greenland Ice Sheet which expanded and retreated across the continental shelf offshore of SE Greenland during, and following, the last glacial maximum. An ancestral Kangerlussuaq Glacier flowed along Kangerlussuaq Trough, a cross shelf bathymetric trough which extends from the mouth of Kangerlussuaq Fiord to the edge of the continental shelf, where it terminates in a trough-mouth fan. Streamlined subglacial bedforms record convergent ice flow into the trough. Sediment cores from along the trough recovered subglacial tills recording a grounded ice sheet. The tills are overlain by a range of deglacial, glacimarine facies recording ice sheet retreat by melting and iceberg calving. A suite of new radiocarbon dates were obtained on foraminifera and shells from the deglacial facies in a transect of cores extending from the trough-mouth fan to the inner shelf. The dates constrain the timing of initial retreat from the outer shelf and allow the position of the grounding-line to be tracked during retreat. The new radiocarbon dates significantly improve the offshore temporal constraints on the post-LGM deglaciation for this sector of the Greenland Ice Sheet and, allied with core sedimentology and foraminferal assemblage data, allow assessment of the role of ocean warming in driving retreat of the ancestral Kangerlussuaq Glacier.

 

How to cite: O'Cofaigh, C., Hunt, M., Lloyd, J., Hogan, K., Snowman Andresen, C., Larter, R., and Roberts, D.: Deglaciation of the ancestral Kangerlussuaq Glacier from the continental shelf offshore of SE Greenland following the LGM, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14254, https://doi.org/10.5194/egusphere-egu26-14254, 2026.

EGU26-14737 | ECS | Orals | CR1.4

Two million years of the Eurasian Ice Sheet 

Kaleb Wagner, Lotta Ylä-Mella, Martin Margold, Mads Faurschou Knudsen, and John D. Jansen

Reconstructions of Northern Hemisphere ice sheets throughout the Quaternary are central to interpreting past variations in sea level, ocean-atmospheric circulation, and climate. Yet, terrestrial records of the earliest glaciations are fragmentary and anchored principally to relative chronostratigraphic frameworks, limiting direct comparison with more continuous marine archives. Here, we present new dating and sedimentary provenance constraints, motivating reassessment of the early history of the Eurasian Ice Sheet (EIS) and its role within the evolving Pleistocene climate system.

Cosmogenic 26Al-10Be burial dating of key glacigenic deposits from northwest and central Europe reveals that extensive EIS advances occurred repeatedly during the Early Pleistocene, beginning as early as ~2.35 million years ago (Ma), and substantially predating the traditionally inferred onset of lowland glaciation during marine isotope stages (MIS) 16–12 (~0.65–0.45 Ma). Detrital zircon U-Pb fingerprinting of these deposits indicates that successive EIS advances transported sediment from the Fennoscandian Shield into the North Sea Basin and the North European Plain, implying that ice flow pathways through the Baltic Depression were established already in the Early Pleistocene and the Baltic (Eridanos) River System had terminated by at least ~1.5 Ma.

Our revised chronologies highlight that the most extensive EIS configurations formed prior to the Middle Pleistocene Transition, and within the context of apparent low-amplitude glacial cycles of the ‘41-kyr world.’ When integrated with independent geochronologic evidence from North America, these findings (within uncertainties) point to broadly synchronous Early–Middle Pleistocene expansions of the major Northern Hemisphere ice sheets. Such early attainment of continental-scale ice sheets may help to reconcile available terrestrial evidence with emerging reconstructions of significant glacial sea-level lowstands prior to the dominance of ~100-thousand year glacial cycles.

More generally, this synthesis calls for re-examination of long-standing European Quaternary stratigraphic frameworks and suggests that Eurasian glaciation may have played an important role in reorganizing continental drainage, modulating freshwater delivery to the North Atlantic, and influencing ocean-atmospheric circulation throughout the Early–Middle Pleistocene.

How to cite: Wagner, K., Ylä-Mella, L., Margold, M., Faurschou Knudsen, M., and D. Jansen, J.: Two million years of the Eurasian Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14737, https://doi.org/10.5194/egusphere-egu26-14737, 2026.

EGU26-15366 | ECS | Orals | CR1.4

The case for Ross Bank ice rises since the middle Miocene 

William Weber and Philip Bart

Many tens of ice rises exist at the marine margins of the Antarctic Ice Sheet.  Isle-type ice rises in particular are those where an ice shelf is pinned to an underlying submarine bank.  Recent and ongoing studies show that Ross Bank, on the middle continental shelf of central Ross Sea, was the former site of an important Ross Ice Shelf ice rise during the advance and retreat of the West Antarctic Ice Sheet (WAIS) in the last glacial cycle.  Ross Bank is a broad and anomalously shallow water platform whose crest rises to 150 m water depth. Despite its importance as a buttressing site, little is known about how, when and why such submarine banks formed. Here, we use a grid of seismic data acquired during expedition NBP2301/2 to reconstruct how Ross Bank morphology evolved.  Our seismic-based correlations and mapping show that Ross Bank overlies the western flank of the Central High, a large basement horst created during the rifting of Ross Sea.  Seismic correlation to lithologic and chronologic control at IODP expedition 374 sites U1521 and U1522 indicates that thick grounding zone wedges were deposited at the site of Ross Bank during the early Miocene.  Intermittent advance of erosive ice streams deeply eroded those wedges and produced approximately 400 meters of relief at Ross Bank prior to the middle Miocene.  The complete absence of middle Miocene strata at Ross Bank suggests significant intervals of subglacial erosion associated with glacial stages of the Middle Miocene Shift.  In the time since, relatively minor aggradation on the crest of Ross Bank occurred during parts of the late Miocene, Pliocene and Pleistocene. Our analyses make the case that a shallow submarine area existed at Ross Bank since the middle Miocene.  The bank would have been the site of ice rises that influenced the advance and retreat of the WAIS in central Ross Sea over the past 14 Myr.

How to cite: Weber, W. and Bart, P.: The case for Ross Bank ice rises since the middle Miocene, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15366, https://doi.org/10.5194/egusphere-egu26-15366, 2026.

EGU26-15518 | Orals | CR1.4

GLAC3 rates and phasing: the first joint history matching of global last glacial cycle ice sheet evolution and regional earth rheology 

Lev Tarasov, April Dalton, Art Dyke, Marilena Geng, Alexis Goffin, Anna Hughes, Benoit Lecavalier, Jan Mangerud, Glenn Milne, John-Inge Svendsen, and Sarah Woodroffe

GLAC3 is the first history matching of every last glacial cycle ice sheet. It therefore includes North American, Greenlandic, Icelandic,
Eurasian, Tibetan, Patagonian, and Antarctic components. Instead of determining a non-robust "optimal" chronology, history matching aims
to "bound reality" with robust assessment of both proxy data and model (both parametric and structural) uncertainties. For the four major ice
sheets, this entails Bayesian artificial neural network emulation of the glaciological model predictions to enable adequate Markov Chain
Monte Carlo sampling of chronologies. The history matching is against a large set of geophysical (such as relative sea level and marine
limit), geological (cosmogenic exposure and C14 ages), and glaciological (such as present-day ice surface velocity) constraints.

Aside from being a product of history matching, GLAC3 has two additional unique features. Firstly, it is the only available
deglacial, let alone full glacial cycle, global set of chronologies from glaciological modelling, using the Glacial Systems Model
(GSM) with hybrid shallow ice and shallow shelf ice dynamic. This enables physical resolution of ice sheets, ice streams, ice shelves,
and grounding line migration. As such, GLAC3 is subject to glaciological constraints such as borehole temperature profiles that
non-glaciological reconstructions can't resolve. Secondly, the glaciologically modelling is self-consistently coupled with full
visco-elastic glacio-isostatic adjustment enabling joint history matching of ice history and regional earth viscosity.

The presentation will focus on the relative phasing of each ice sheet, rates of mass gain and loss, and rates of ice margin migration. This
will be compared against both far-field relative sea level records as well as the results of fully coupled ice and climate modelling of the
last glacial cycle with LCice (LOVECLIM + GSM).

How to cite: Tarasov, L., Dalton, A., Dyke, A., Geng, M., Goffin, A., Hughes, A., Lecavalier, B., Mangerud, J., Milne, G., Svendsen, J.-I., and Woodroffe, S.: GLAC3 rates and phasing: the first joint history matching of global last glacial cycle ice sheet evolution and regional earth rheology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15518, https://doi.org/10.5194/egusphere-egu26-15518, 2026.

Reconstructing the precise timing and geometry of the British-Irish Ice Sheet (BIIS) is critical for understanding the sensitivity of the North Atlantic climate system to abrupt perturbations. We present preliminary results from a cosmogenic beryllium-10 (10Be) surface-exposure chronology of glacial deposits in the Gaddagh valley, situated on the northern flank of the McGillycuddy’s Reeks, southwest Ireland. Our geomorphological and chronological transect reveals a detailed history of deglaciation and ice-margin fluctuations since the Late Pleistocene.

Initial results indicate that high-elevation areas (300–350 m asl) adjacent to the main valley were ice-free by ~28 ka (n=2), suggesting an earlier onset of local thinning than previously modelled. The prominent "Hag’s Tooth Moraine”, the primary geomorphological feature in the valley, appears to represent a culmination during the Last Glacial Maximum (LGM). Following this peak, the deposition of a barely preserved subdued moraine impounded Loch Callee at ~19 ka (n=3), marking a significant phase of ice retreat at the onset of Termination 1. The final pulse of glacial activity is recorded 200 m higher in the catchment by a complex of five latero-frontal moraines. These landforms mark the former extent of a small cirque glacier, with the final abandonment of these positions occurring at ~12.7 ka (n=3).

Thus far, our findings implicate the following. First, the data do not support a complete ice cover over the McGillycuddy’s Reeks during the LGM as previously proposed; instead, we suggest that ice was topographically restricted to the main valleys, with the front of the Gaddah glacier not below 150 m asl. Second, our chronology indicates that terminal deglaciation occurred during a period traditionally associated with relatively cold climate conditions. This pattern of glacier recession during inferred year-round cold climate aligns with recent 10Be chronologies from Scotland (Bromley et al., 2018, 2023), central East Greenland (Kelly et al., 2025), southernmost Greenland (Carlson et al., 2021) and Norway (Putnam et al., 2023; Wittmeier et al., 2020), which demonstrate glacier shrinkage during the Younger Dryas. These results contribute to the ongoing discussion about glacier extension in the area and the evolving paradigm of North Atlantic climate dynamics, emphasizing the role of summer temperature as the primary driver of glacial mass balance during millennial-scale stadials.

 

How to cite: Rodriguez, P. and Bromley, G.: Lateglacial deglaciation of the McGillycuddy’s Reeks, SW Ireland through 10Be surface-exposure dating of glacial deposits in the Gaddah Valley: Implications for late glacial climate variability., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15730, https://doi.org/10.5194/egusphere-egu26-15730, 2026.

EGU26-16257 | ECS | Orals | CR1.4

Evidence and implications of rapid early-Holocene thinning of Scott Glacier, East Antarctica 

Corey Port, Richard Jones, Andrew Mackintosh, Levan Tielidze, Reka Fulop, Klaus Wilcken, Tyler Pelle, Duanne White, and Jacinda O'Connor

The East Antarctic Ice Sheet is showing evidence of mass loss, particularly near its coastal margin in the Wilkes and Aurora Subglacial Basins, and at Denman Glacier. Quantitative satellite observations indicate significant grounding line retreat at these sites, suggesting potential vulnerability to Marine Ice Sheet Instability. Reconstructions of past ice sheet behaviour using cosmogenic exposure dating can provide robust geological constraints on prior ice sheet thinning. This helps us assess whether contemporary thinning and retreat is unprecedented, while also establishing a geologically constrained precedent for ice-sheet behaviour and sensitivity to which projections can be compared.

Here we present the first reconstruction of Holocene thinning of Scott Glacier, East Antarctica, located 56 km east of Denman Glacier. Scott Glacier is currently stable, pinned by subglacial topography, though is projected to retreat into the Denman trough, and ultimately contribute to the instability of the Denman-Scott System. Together, the Denman and Scott Glacier could contribute up to 1.5 m to global sea level rise if fully deglaciated. To examine its past behaviour, we collected 11 bedrock and erratic samples over an elevation transect at Grace Rocks (-66.421S, 100.508E), an ice-free nunatak adjacent to the modern-day grounding line. Exposure ages were then derived from measured cosmogenic Berilyum-10 and in-situ Carbon-14 concentrations. Together, they provide consistent evidence for rapid thinning during the early-Holocene, with estimates suggesting a maximum thinning rate of ~1 m/yr, comparable to thinning observed in parts of the ice sheet today. This thinning history provides robust geological constraints on the past behaviour and sensitivity of Scott Glacier, and a baseline from which to assess its contemporary and projected retreat and vulnerability.

We also derive projections of ice elevation change at Scott Glacier from simulations with the Ice-sheet and Sea-level System Model (ISSM). Projections show thinning rates exceeding 2 m/yr over the next two centuries across the Denman-Scott region, with an average thinning rate of 0.65 m/yr at Grace Rocks projected until 2085. While there are uncertainties associated with these models, the rates and sensitivity we established from the early-Holocene geological record suggest that modelled changes of this magnitude are plausible, and that despite contemporary stability, Scott Glacier is at risk of contributing significantly to regional icesheet instability and sea level rise in coming decades to centuries.

How to cite: Port, C., Jones, R., Mackintosh, A., Tielidze, L., Fulop, R., Wilcken, K., Pelle, T., White, D., and O'Connor, J.: Evidence and implications of rapid early-Holocene thinning of Scott Glacier, East Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16257, https://doi.org/10.5194/egusphere-egu26-16257, 2026.

EGU26-16822 | ECS | Orals | CR1.4

Constraining subglacial erosion in Greenland using estimates of fjord sediment volumes and ice-flow modeling 

Jonas Damsgård, Caroline Brand, Gustav Jungdal-Olesen, and Vivi Pedersen

Fjord landscapes along the margins of past and present ice sheets testify to the significant long-term erosive power of large outlet glaciers. Yet, our understanding of the rates and processes of subglacial erosion and sediment transport beneath ice sheets remains incomplete. Quantifying these processes is crucial for reconstructing past ice dynamics, estimating sediment fluxes to the ocean, and understanding long-term landscape evolution.

Greenland’s narrow, steep-sided fjords act as natural sediment traps, preserving erosion products delivered by large outlet glaciers during deglaciation. These fjord sediments constitute a valuable constraint on past erosion rates and glacial sediment fluxes when combined with ice catchment areas and retreat histories in a source-to-sink framework. However, most Greenlandic fjords remain unmapped in terms of sediment thickness because sediment cores rarely penetrate deeply and seismic data acquisition is sparse. In contrast, accurate bathymetric data are increasingly available for many fjords. We use a geomorphological approach to estimate sediment infill volumes based on fjord cross-sectional profiles, where deviations from the expected U-shape and the slope of the sidewalls are used to infer sediment thickness.

We quantify fjord infill volumes for several fjords and use these to estimate average catchment-wide erosion rates. The timing of deposition (starting when the ice retreated into the fjord) is constrained by available deglaciation models. To further explore the temporal and spatial variability of subglacial erosion, we employ a coupled ice-flow and erosion model (iSOSIA), driven by paleoclimate forcing, to simulate erosion beneath marine-terminating outlet glaciers during the last deglaciation (~21–0 ka BP). Modeled sediment outputs are compared with our estimates of sediment volumes and accumulation rates from sediment cores to calibrate the model erosion parameters.

Our results indicate that average deglacial erosion rates are largely independent of catchment size but vary significantly through time and space within ice-sheet catchments. Rates can exceed 10 mm yr⁻¹ for topographically steered, fast-flowing outlet glaciers, while much lower rates (<0.1 mm yr⁻¹) occur in slower-flowing interior regions with slow-moving ice. Quantifying and linking offshore sediment volumes with numerical modeling provides an opportunity to constrain subglacial erosion rates, sediment transport and ice-sheet reconstructions. This work demonstrates the value of integrating glaciological modeling with marine sediment archives to refine erosion estimates and improve predictions of future sediment fluxes under continued ice-sheet retreat.

How to cite: Damsgård, J., Brand, C., Jungdal-Olesen, G., and Pedersen, V.: Constraining subglacial erosion in Greenland using estimates of fjord sediment volumes and ice-flow modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16822, https://doi.org/10.5194/egusphere-egu26-16822, 2026.

EGU26-18150 | ECS | Posters on site | CR1.4

Dynamics of the British-Irish Ice Sheet in the South of Ireland. 

Apolline Mariotti, Helen Dulfer, Margaret Jackson, and Samuel E. Kelley

Accurate reconstructions of past ice sheet dynamics are essential for constraining ice sheet sensitivity to climate forcing and projecting future sea-level rise in a warming climate. The British-Irish Ice Sheet (BIIS) during the Last Glacial Maximum presents a critical test case, and yet, reconstructions of its southern margin across Ireland differ fundamentally in both extent and timing.
 
Earlier geomorphic mapping-based models proposed an ice-free corridor across southern Ireland during the last glacial period. In contrast, more recent offshore and near-shore sediment-based reconstructions propose a maximum BIIS extent covering the entire island and extending to the continental shelf edge, requiring an ice sheet thick enough to override most Irish mountain ranges. This interpretation conflicts with evidence for localized mountain glaciation in the same time period in areas like the Wicklows Mountains, which would have been impossible under a thick ice sheet. The scarcity of reliable terrestrial geochronological control points (e.g., cosmogenic exposure ages, OSL, 14C) in southern Ireland significantly contributes to these uncertainties, thus limiting the accuracy of reconstructions of BIIS expansion and retreat.
 
This project aims to resolve these contradictions by providing robust chronological control on the position of the BIIS margin in the south of Ireland. We conducted sampling campaigns in three critical locations: the Wicklow Mountains, the Comeragh Mountains, and the Kerry Peninsula. Our sampling strategy targeted boulders at multiple elevations and aspects to capture both the timing and geometry of ice cover. We present preliminary 10Be surface-exposure ages from erratic boulders in the Comeragh Mountains (maximum elevation 792 m), sampled on transects from the northern, eastern, southern, and western slopes.
 
These chronological constraints will refine deglaciation scenarios for the BIIS southern margin, in turn improving our understanding of regional landscape evolution, and provide empirical data for testing ice sheet models under past climate conditions similar to future warming scenarios.

How to cite: Mariotti, A., Dulfer, H., Jackson, M., and Kelley, S. E.: Dynamics of the British-Irish Ice Sheet in the South of Ireland., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18150, https://doi.org/10.5194/egusphere-egu26-18150, 2026.

EGU26-20495 | ECS | Orals | CR1.4

Using reconstructed ice streams to calibrate a coupled climate-ice-sheet model of the North American Ice Sheet Complex during the Last Glacial Maximum  

Yvan Romé, Lauren Gregoire, Niall Gandy, Violet Patterson, and Jeremy Ely

Coupled climate-ice-sheet modelling provides critical insights into the mechanisms underlying ice-sheet-climate feedback. These processes have strong implications for past and future climate change events, yet modelling efforts remain constrained by uncertainties in key model parameters. To address this limitation, we rely on comparisons between model outputs and available records of past ice sheets. Historically, this involved matching simulated ice sheets to reconstructed extent and volume derived from a range of geomorphological and sea level change data. Although these metrics are useful to validate ice sheet geometry and volume, they only provide limited information on ice sheet dynamics. New methods, which compare the footprint of reconstructed and simulated palaeo-ice streams, offer promising ways to incorporate a dynamical dimension into model calibration (Ely et al., 2024, Journal of Quaternary Science). 

In this project, we catalogue the distinct dynamical configurations observed in an ensemble of coupled climate-ice-sheet simulations of the Last Glacial Maximum (LGM, 21,000 years ago). This ensemble includes 124 equilibrium simulations generated using the coupled atmosphere-ice-sheet model FAMOUS-BISICLES, with variation applied to 12 model parameters representing ice dynamics, albedo and climate feedbacks (Patterson et al., 2025, EGUsphere). The ice sheet dynamics not only assess the model’s ability to replicate the LGM reconstructions of the Laurentide ice streams (Margold et al. 2018, Quaternary Science Reviews), but they also inform the sensitivity of the simulated ice sheets to climate forcing.  

Plausible simulations of the North American ice sheets in terms of volume and extent can be obtained across various regions of the parameters space, resulting in significant discrepancies in potential ice streaming patterns. Surface Mass Balance (SMB) is the main factor behind these changes in dynamical configurations: simulations with low accumulation tend to produce less numerous and intense ice streams, whereas high accumulation is associated with more vigorous ice streaming. In addition, the parametrisation of the ice dynamics influences the location and consistency of the ice streams, as well as the ability of the ice sheet to respond to climate change events. 

We find that simulations with relatively high SMB and ice dynamics parameters that enable fast-flowing and well-defined ice streams best match estimates of Last Glacial Maximum North American ice sheet extent, volume and ice stream location. Conversely, high friction coefficients and porous subglacial till, or low resolution of the ice sheet margins and the bedrock topography, result in ice stream patterns that are inconsistent with reconstructions and less responsive to climate forcing. This work demonstrates the relevance of comparison between reconstructions of past ice streams and model simulations to provide strong constraints on dynamical ice sheet models and ice sheet sensitivity to climate changes.

How to cite: Romé, Y., Gregoire, L., Gandy, N., Patterson, V., and Ely, J.: Using reconstructed ice streams to calibrate a coupled climate-ice-sheet model of the North American Ice Sheet Complex during the Last Glacial Maximum , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20495, https://doi.org/10.5194/egusphere-egu26-20495, 2026.

EGU26-20734 | ECS | Posters on site | CR1.4

Holocene evolution of the Amundsen Sea sector from three-dimensional modelling constrained by extensive ice-penetrating radar isochrones 

Julien A. Bodart, Johannes C.R. Sutter, Duncan A. Young, Donald D. Blankenship, Vjeran Višnjević, Antoine Hermant, and Emma Spezia

Whilst our understanding of the past ice-sheet extent of the Amundsen Sea sector at the Last Glacial Maximum (LGM) is relatively well known, the subsequent retreat (and potential re-advance) of Pine Island and Thwaites glaciers during the Holocene is contrastingly less understood. Some studies conducted across its neighbouring catchments, such as the Weddell and Ross Sea sectors, indicate that the grounding line may have retreated beyond its current position, and then subsequently re-advanced primarily due to isostatic rebound and stabilisation around pinning points. Over the Amundsen Sea sector, contrasting evidence suggests that non-linear changes in inland ice-sheet cover may have occurred, but little evidence exists for large changes affecting the continuous and gradual retreat of the grounding line from the LGM to its current position today. Here, we employ the three-dimensional PISM ice-sheet model to reconstruct the evolution of this sector since the LGM. We first explore the full parameter space using a Latin Hypercube Sampling method, and further constrain our best sets of simulations using extensive and newly available isochronal surfaces imaged by radars and dated at several snapshots throughout the last ~20 thousand years. We show that isochrones are essential for assessing the transient evolution of paleo simulations, particularly in off-divide areas of the ice sheet, and discuss how different geothermal heat-flux and SMB datasets impact the transient evolution of this sensitive sector.

How to cite: Bodart, J. A., Sutter, J. C. R., Young, D. A., Blankenship, D. D., Višnjević, V., Hermant, A., and Spezia, E.: Holocene evolution of the Amundsen Sea sector from three-dimensional modelling constrained by extensive ice-penetrating radar isochrones, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20734, https://doi.org/10.5194/egusphere-egu26-20734, 2026.

EGU26-20850 | Posters on site | CR1.4

IN SITU COSMOGENIC 10Be AND 14C: A WINDOW INTO PAST ICE SHEET THICKNESS IN SCOTLAND AND IRELAND 

Samuel E. Kelley, Clara Crowell, Nathaniel Lifton, and Simon Pendleton

The British-Irish Ice Sheet (BIIS) is one of the best-constrained paleo-ice sheets in the world, with detailed geomorphological and geochronological data constraining margins and retreat patterns. Despite this, the thickness of this former ice sheet remains uncertain. High elevation locations offer potential for constraining former ice sheet thickness; however, a lack of glacial erosion due to cold-based ice cover of mountain summits limits the use of single isotope cosmogenic exposure dating, as inherited nuclides commonly yield ages older than the last glaciation from mountain top landscapes. As such, landscapes that experienced cold-based ice cover and those at relatively high elevations are underrepresented in glacial reconstructions, both for the BIIS and globally, thus negatively affecting their ability to serve as training datasets for numerical models used to reconstruct paleo-ice masses. Here, we use paired 10Be/14C extracted from bedrock and boulder samples in high-elevation locations across Scotland and Ireland. Our multi-nuclide approach uses one long-lived nuclide, 10Be, and one short-lived nuclide, 14C, allowing for an examination of two questions: 1) What is the vertical pattern of deglaciation across the BIIS? 2) Did mountaintops exist as nunataks during the last glaciation? To address these questions, we collected samples from one site in Scotland (Cairngorm Mountains) and four Irish mountains (Dublin, Wicklow, and Mourne Mountains, as well as Mt. Brandon in Dingle) for paired 10Be and 14C analysis, yielding 22 new pairs of exposure ages. At four of our study sites, 10Be results yield exposure ages preceding the LGM, indicative of a lack of erosion during the last glaciation or prolonged exposure. Our 14C results show concentrations at or near secular equilibrium at three of those sites, indicating either exposure during the last glaciation or a period of glaciation too short for inherited 14C to decay. These results provide insight into ice-mass thinning and the spatial pattern of glacial erosion, allowing for a more holistic view of cryospheric change in the region in response to a changing climate.

How to cite: Kelley, S. E., Crowell, C., Lifton, N., and Pendleton, S.: IN SITU COSMOGENIC 10Be AND 14C: A WINDOW INTO PAST ICE SHEET THICKNESS IN SCOTLAND AND IRELAND, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20850, https://doi.org/10.5194/egusphere-egu26-20850, 2026.

EGU26-2716 * | ECS | PICO | CR1.5 | Highlight

Peak glacier extinction in the mid-twenty-first century 

Lander Van Tricht, Harry Zekollari, Matthias Huss, David Rounce, Lilian Schuster, Rodrigo Aguayo, Patrick Schmitt, Fabien Maussion, Brandon Tober, and Daniel Farinotti

Recognising the global importance and vulnerability of mountain glaciers, the United Nations General Assembly declared 2025 the International Year of Glaciers’ Preservation, highlighting the critical role of glaciers in the hydrological cycle and the growing societal risks associated with their rapid decline. These concerns are well founded: glaciers worldwide are retreating rapidly, yet projections have traditionally focused on changes in mass and area rather than on the fate of individual glaciers.

Here, we quantify the future evolution of the global number of glaciers and introduce the concept of peak glacier extinction: the year in which the largest number of individual glaciers is projected to disappear. Using three global glacier models and the Randolph Glacier Inventory v6.0, we project the fate of more than 200,000 glaciers worldwide under four policy-relevant global warming scenarios by 2100 (+1.5 °C, +2.0 °C, +2.7 °C and +4.0 °C relative to pre-industrial levels). A glacier is classified as extinct when its area falls below 0.01 km² or its remaining volume declines to less than 1% of its initial value.

Across all scenarios, we identify a pronounced mid-century peak in glacier extinction. Under a +1.5 °C pathway, this peak occurs around 2041, with approximately 2,000 glaciers disappearing per year, whereas under a +4.0 °C scenario it shifts to the mid-2050s and intensifies to nearly 4,000 glacier extinctions annually. Regional differences reflect contrasts in glacier size distributions and climatic conditions. Our results highlight the urgency of ambitious climate action. Whether the world faces the loss of 2,000 or 4,000 glaciers per year by mid-century, and whether roughly 20,000 or 100,000 glaciers remain by the end of the century, will be determined by near-term policy and societal choices made today.

How to cite: Van Tricht, L., Zekollari, H., Huss, M., Rounce, D., Schuster, L., Aguayo, R., Schmitt, P., Maussion, F., Tober, B., and Farinotti, D.: Peak glacier extinction in the mid-twenty-first century, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2716, https://doi.org/10.5194/egusphere-egu26-2716, 2026.

EGU26-5383 | ECS | PICO | CR1.5

FROST in the European Alps – Implementing a data assimilation framework for calibration of surface mass balance models. 

Oskar Herrmann, Veena Prasad, Anna Zöller, Alexander R. Groos, Samuel Cook, Christian Sommer, and Johannes J. Fürst

The demise of glaciers in the European Alps appears inevitable. The remaining question is the rate of ice loss and the timing of complete disappearance. This is particularly important for local water resource management and hazard assessment. Answering this requires glacier models that can robustly project glacier evolution over the coming decades. With the Instructed Glacier Model (IGM), an important tool for such projections has been made available, enabling computationally efficient modeling of glaciers as three-dimensional objects.

The remaining task is to accurately calibrate the glacier model. Fortunately, major advances in remote sensing provide an unprecedented amount of satellite observations that can be used for calibration on regional to global scale, even in remote areas without in-situ observations. The Framework for assimilating Remote-sensing Observations for Surface mass balance Tuning (FROST) utilizes a global elevation change product to infer equilibrium line altitudes and surface mass balance gradients. We tested the framework on 409 individual glaciers in the European Alps that were larger than 1 km² at the beginning of the century and evaluated the results against in situ measurements and end-of-summer snow line altitudes. The results show that the calibrated equilibrium line altitudes agree well with the snow line altitudes, while the surface mass balance gradients differ from glaciological measurements. This discrepancy is partially explained by the presence of small glaciers, which challenge gradient-based surface mass balance models, and by uncertainties of observation that lead to inaccurately modelled glacier flow. The first regional application of FROST shows promising results, provides meaningful insights and reveals challenges  for glacier projections in central Europe.

How to cite: Herrmann, O., Prasad, V., Zöller, A., Groos, A. R., Cook, S., Sommer, C., and Fürst, J. J.: FROST in the European Alps – Implementing a data assimilation framework for calibration of surface mass balance models., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5383, https://doi.org/10.5194/egusphere-egu26-5383, 2026.

EGU26-5777 | ECS | PICO | CR1.5

Monitoring and forecasting the state of Svalbard’s cryosphere using a digital twin (SvalbardDT) 

William D. Harcourt, Morag Fotheringham, Georgios Leontidis, Aiden Durrant, Ashley Morris, Eirik Malnes, Robert Ricker, Adrian Luckman, Ward Van Pelt, Veijo Pohjola, Livia Jakob, and Noel Gourmelen

In this contribution, we will demonstrate the first prototype of the Svalbard cryosphere digital twin (SvalbardDT v1; https://svalbarddt.org/), which is a Digital Twin Component of ESAs Digital Twin Earth (DTE). An environmental digital twin observes a physical entity (i.e. the cryosphere), fuses multi-modal observations together, then generates what if scenarios to improve human decision-making. In this way, there are two-way flows of information (i.e. data) between the physical and digital assets. In Svalbard, where rates of warming are six times faster than the global average, digital twins have the potential to be used by researchers to analyse trends in the cryosphere, by local communities to improve navigation, and by policy-makers to improve decision-making. Furthermore, Svalbard is considered a ‘super site’ of in situ observations in a pan-Arctic context owing to the permanent infrastructure and long history of international scientific collaboration on the archipelago, hence it is a prime location to develop Arctic digital twin technology. Here, we will provide a demonstration of the capabilities of SvalbardDT version 1 as a new tool for monitoring Svalbard’s cryosphere in the 21st century (2010-present), the underlying architecture, and the next steps towards full operationalisation.

SvalbardDT represents a digital twin of Svalbard’s cryosphere covering glaciers, snow and sea ice observed through a combination of Earth Observation data sets and reanalysis data products. These data products are multi-modal i.e. they are collected at different resolutions, scales and time/spatial periods. SvalbardDT fine-tunes a deep learning foundational model to ingest the relevant data products and harmonise them into a 4D data cube describing the data set variable, x-dimension, y-dimension, and its changes over time. This produces weekly to monthly data cubes describing ~21 parameters. SvalbardDT focuses on the application of two case studies which are accessed through an online dashboard: (1) exploring the current state of cryosphere conditions in Svalbard to simulate terrestrial and marine navigation routes across the archipelago; and (2) forecast extreme Rain on Snow and Ice (ROSI) events using an AI foundation model. The associated toolboxes help to improve our understanding of the interconnecting processes shaping glaciers and ice caps across Svalbard.

How to cite: Harcourt, W. D., Fotheringham, M., Leontidis, G., Durrant, A., Morris, A., Malnes, E., Ricker, R., Luckman, A., Van Pelt, W., Pohjola, V., Jakob, L., and Gourmelen, N.: Monitoring and forecasting the state of Svalbard’s cryosphere using a digital twin (SvalbardDT), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5777, https://doi.org/10.5194/egusphere-egu26-5777, 2026.

EGU26-7409 | ECS | PICO | CR1.5

Lagged glacier response to past climate forcing and its role in recent volume loss 

Magali Ponds, Rodrigo Aguayo, and Harry Zekollari

Glaciers are currently losing mass at unprecedented rates. These losses are often attributed to past climate forcing. However, a substantial share of glacier volume loss reflects the delayed adjustment of glacier geometry to past climate conditions. This lag arises because glacier geometry can evolve only as fast as ice can flow and surface mass balance can add or remove ice, making glacier change a continual race to adapt to changing climatic conditions.

In this study, we globally quantify the fraction of glacier volume loss that is committed to past climate forcing, relative to losses driven by concurrent climate conditions. Using the Open Global Glacier Model (OGGM), we decompose volume loss over the preceding decade for reference years. Each period is simulated twice: once forced by the climate of the reference period and once with the climate from a preceding period. This allows us to isolate the fraction of volume loss attributable to committed adjustment. Preliminary results indicate that of the 4.5% global glacier volume loss between 2000 and 2019, approximately 90% would also have occurred under the climate conditions of 2000–2010 alone, and nearly half can be attributed to climate conditions from 1990–2000.

Our results provide a new perspective on the evolving balance between glacier geometry and climate forcing, enabling a clearer interpretation of recent glacier change and its underlying drivers.

How to cite: Ponds, M., Aguayo, R., and Zekollari, H.: Lagged glacier response to past climate forcing and its role in recent volume loss, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7409, https://doi.org/10.5194/egusphere-egu26-7409, 2026.

EGU26-11039 | ECS | PICO | CR1.5

One mass balance model to rule them all: joint assimilation of remote sensing and glaciological data into MassBalanceMachine 

Alban Gossard, Jordi Bolibar, Marijn van der Meer, and Kamilla Hauknes Sjursen

Glacier surface mass balance observations are highly heterogeneous, with point glaciological measurements spanning decadal timescales being limited to a few well-monitored regions, while geodetic observations are available globally with a multi-annual baseline and almost full glacier coverage. Existing surface mass balance modelling approaches can only calibrate their parameters for individual glaciers or regions with available observations. This often implies that a big part of the available observations per glacier (generally glaciological data) cannot be exploited for calibration since they play the role of independent data for validation. There is a need to move towards flexible surface mass balance models, capable of leveraging in a coherent fashion both glaciological and remote sensing data.

To address this challenge, we introduce a new version of MassBalanceMachine, a neural network-based model that predicts monthly surface mass balance using topographical features and monthly climate forcing as inputs. The pointwise nature of the model, combined with the global availability of input features thanks to OGGM and ERA5, enables the implementation of custom loss functions to train the model. This loss function allows the model to align with both glaciological measurements and geodetic mass balance observations over multiple decades.

By leveraging the interannual variability and point-wise nature from glaciological data and correcting long term biases with geodetic data, MassBalanceMachine can generate reliable high-resolution monthly mass balance predictions for unmonitored glaciers, and correct existing predictions where previous training strategies are known to fail, e.g. in the Alps. This approach exploits data from data-rich sparse regions to make predictions for other unmonitored regions or glaciers, offering a scalable solution for global glacier mass balance estimation.

How to cite: Gossard, A., Bolibar, J., van der Meer, M., and Hauknes Sjursen, K.: One mass balance model to rule them all: joint assimilation of remote sensing and glaciological data into MassBalanceMachine, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11039, https://doi.org/10.5194/egusphere-egu26-11039, 2026.

EGU26-11494 | PICO | CR1.5

Cool no More! Mountain Glaciers Recouple to Atmospheric Warming over the Twenty-First Century 

Thomas Shaw, Evan Miles, Michael McCarthy, Pascal Buri, Nicolas Guyennon, Franco Salerno, Luca Carturan, Benjamin Brock, and Francesca Pellicciotti

Warm atmospheric conditions promote the rise of local microclimates over mountain glaciers and the generation of cool katabatic winds. These “Glacier winds” act to reinforce a shallow boundary layer above melting snow and ice in the summer months, mediating their response to temperature fluctuations in the wider mountain domain. Recent observational studies have highlighted the magnitude to which these temperature fluctuations over glaciers are decoupled from broader temperature changes, promoting cooling that can slow down melting. Nevertheless, they have largely drawn upon individual glacier case studies with little broader quantification of its scale and relevance for glaciers response to climate change.

 

We compiled meteorological observations from > 350 on-glacier automatic weather station records from >60 glaciers around the world over the past three decades. We contrast the air temperature conditions on-glacier with local, off-glacier weather station records to find that above-ice air temperatures warms ~0.73°C on average for every 1°C change in the surrounding mountain atmosphere. Using a combination of available meteorological and topographical data for each glacier in our dataset, we build a statistical model to estimate the magnitude of cooling over mountain glaciers globally. A global estimate of near-surface cooling over mountain glaciers based upon ERA5-Land climatologies for 2000-2022 reveals stark regional variability in how glaciers ‘feel’ temperature warming in the mountains. We demonstrate that larger glaciers in warmer and more humid environments maintain stronger and more persistent glacier winds that promote greater localised cooling. In contrast, on small, fragmenting glaciers in drier environments, especially those where exposure to synoptic winds or increased debris cover is common, glacier winds and localised cooling are limited.  

 

We leverage ensemble climate estimates from socio-economic pathway SSP2-4.5 and SSP5-8.5 scenarios of sixth phase of the Coupled Model Intercomparison Project (CMIP6) as well as published estimates of glacier volume loss until 2100 to provide a first estimate of the expected future glacier cooling under a warmer climate. While glacier winds are expected to increase near-surface cooling under a warmer climate of the 2030’s and 2040’s in several glacier regions of the world, widespread glacier retreat will limit the development of these glacier winds and, ‘recouple’ temperature variability over glaciers to their surroundings and thus enhance the sensitivity of glaciers to broader climatic warming in the latter half of the 21st century. In the European Alps, it is estimated that the period of maximised glacier katabatic wind development has already passed, signalling the expected demise of cooler meteorological conditions there.

How to cite: Shaw, T., Miles, E., McCarthy, M., Buri, P., Guyennon, N., Salerno, F., Carturan, L., Brock, B., and Pellicciotti, F.: Cool no More! Mountain Glaciers Recouple to Atmospheric Warming over the Twenty-First Century, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11494, https://doi.org/10.5194/egusphere-egu26-11494, 2026.

EGU26-11914 | ECS | PICO | CR1.5

Global glacier change observations (1535–2025) and mass loss (1976–2025) 

Ethan Welty and the WGMS Network

The Fluctuations of Glaciers (FoG) database is the outcome of 130 years of coordinated international glacier monitoring. It is curated by the World Glacier Monitoring Service (WGMS) and regularly updated with observations submitted by a worldwide network of scientific collaborators. Glacier mass, elevation, and length change observations (1535–2025) are complemented by an inventory of glacier-related events (e.g., surges, lake outbursts, and ice avalanches). We will explain the data integration process and evaluate the spatial, temporal, and climatic coverage of the observations.

We will also highlight many enhancements to the database, including structured authorship and bibliographic metadata for each observation, a near-complete full-text archive of all cited literature, glacier names in multiple languages and scripts, the outline used to derive each glacier-wide elevation change, and a representative outline for each in-situ mass change series.

Finally, we will present an annual estimate of global glacier mass loss from 1976 through the 2025 hydrological year. Since 2025, the WGMS combines the latest in-situ mass change observations and remotely-sensed elevation change observations in FoG to calculate a mass-change time series for every glacier on Earth (separate from the Greenland and Antarctic ice sheets) and corresponding regional and global totals.

How to cite: Welty, E. and the WGMS Network: Global glacier change observations (1535–2025) and mass loss (1976–2025), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11914, https://doi.org/10.5194/egusphere-egu26-11914, 2026.

EGU26-12522 | ECS | PICO | CR1.5

Energy and mass balance sensitivities of glaciers to climate across High Mountain Asia 

Evgeny Tumarkin, Thomas Shaw, Achille Jouberton, Shaoting Ren, and Francesca Pellicciotti

Meltwater from High Mountain Asia (HMA) provides water resources to large downstream populations of central, southern and eastern Asia. Recent decades have seen critical changes in the health of the high mountain cryosphere of the region, which poses risks to those dependent upon its water supply. Glaciers of HMA have been observed to change mass at varying rates regionally, likely caused by a combination of heterogeneous climate change and region-specific glacier sensitivities. Regional studies on glacier sensitivities have been limited by computational power to rely on degree day models with higher dependence on calibration and equifinality issues. The same computational limits and data availability have limited energy balance studies to short periods, localised domains or coarsely resolved glacier regions. Explicit representation of glacier specific hypsometry and surface characteristics allows the inclusion of non-linear sensitivity of mass balance with elevation, as well as the inclusion of effects of debris cover. Here we provide a new regional picture of HMA glacier sensitivity to climate using a physically-based high resolution energy and mass balance model (Tethys & Chloris).

We run the model for 50 glaciers in each glacier subregion of HMA, chosen to be representative in terms of glacier area, median elevation, debris area and mean debris thickness. Each glacier is modelled using a clustering of points to discretise its surface, where the number of points is optimised depending on glacier size. We first build a baseline of glacier response to present climate (2000-2010) by forcing the model with bias-corrected hourly ERA5-Land data. For the bias correction, a precipitation factor and temperature bias is optimised for each glacier so that model results match against remotely sensed observations of glacier mass balance, snow line altitude and surface albedo.

To determine glacier sensitivities and their drivers, we perturb temperature and precipitation annually to quantify the mass balance changes at the glacier and regional scale. Further experiments perturbing seasonal climatic signals reveal the relevance and relative impacts of temperature and precipitation changes for regions previously identified as experiencing anomalous mass balance behaviour, such as the Pamir-Karakoram. We analyse the contribution of the main energy fluxes and melt components to the glacier-wide mass balance and quantify the relative influence of precipitation solid fraction and sublimation under these different climate perturbation scenarios. We study the sensitivity of the accumulation area ratio and the glacier equilibrium line altitude as indicators of the regional patterns in glacier health, its year-to-year variability and susceptibility to abrupt shifts under climatic extremes. With this, we identify and explain which regions may be most susceptible to future climate change signals, with an unprecedented attribution to the underlying glacier characteristics and changes in physical processes.

How to cite: Tumarkin, E., Shaw, T., Jouberton, A., Ren, S., and Pellicciotti, F.: Energy and mass balance sensitivities of glaciers to climate across High Mountain Asia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12522, https://doi.org/10.5194/egusphere-egu26-12522, 2026.

EGU26-13047 | ECS | PICO | CR1.5

Reconstructing Annual Global Glacier Mass Balance using Bayesian Neural Fields 

Ritu Anilkumar, Jonathan Bamber, Fabien Maussion, and Michael Zemp

The accelerating loss of glacier mass is disrupting local ecosystems, reshaping hydrological regimes, increasing the likelihood of glacier-related hazards, and undermining the resilience of dependent communities. Quantifying annual glacier mass balance remains challenging because existing estimates rely on either sparse in situ and remote sensing observations or process-based models, each with inherent limitations. Observational approaches, while consistent at global scales, exhibit large regional variations. In contrast, modelling frameworks provide complete spatiotemporal fields but are typically deterministic, sensitive to calibration data, and constrained by assumptions that may overlook key energy balance drivers. Through our approach, we combine the strengths of models and various observational methods in a Bayesian neural network framework. Specifically, we use a Bayesian Neural Field architecture that is first pre-trained on fixed-geometry annual mass balance outputs from the Open Global Glacier Model (OGGM) and then finetuned using multimodal observations available at different spatial and temporal scales. The model uses static glacier characteristics and near-surface climate variables as predictors. We demonstrate through a blocked testing strategy that our framework can fill gaps for glaciers with missing or highly uncertain mass balance records as well as reconstruct meaningful long-term time series. In summary, this approach provides a scalable, uncertainty-aware method for generating spatially and temporally complete annual glacier mass balance estimates.

How to cite: Anilkumar, R., Bamber, J., Maussion, F., and Zemp, M.: Reconstructing Annual Global Glacier Mass Balance using Bayesian Neural Fields, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13047, https://doi.org/10.5194/egusphere-egu26-13047, 2026.

EGU26-14408 | ECS | PICO | CR1.5

Feeling the heat: global detection of volcanic effects on glacier mass balance and dynamics 

Tryggvi Unnsteinsson, Matteo Spagnolo, Brice Rea, Társilo Girona, Iestyn Barr, and Donal Mullan

With the availability of open-access satellite imagery and derived products from open-source tools, global studies of glaciers have become increasingly manageable. Many studies have used these global datasets to delineate spatial and temporal variations in glacier mass balance and dynamics. This has highlighted the effects of seasonal fluctuations and climatic trends on glaciers and has aided the identification of glacier surges. Here we focus on the often-neglected effects volcanoes may have on glacier mass balance and dynamics. First, we analyse the elevation distribution of the world’s glaciers with respect to their proximity to volcanoes and find that there is measurable evidence of the negative mass-balance effect volcanoes have on nearby glaciers. Second, we use the ITS_LIVE glacier velocity dataset along with the new TICOI regularisation and signal decomposition to identify velocity anomalies on glaciers located around volcanoes. This allows us to discern both short-lived velocity anomalies as well as long-term trends and variations in seasonal patterns. We identify multiple velocity anomalies, many of which correlate with climatic trends or weather events, others with surges, but some stand out as volcanically induced. We demonstrate examples of what effect various volcanic processes such as geothermal activity, mass wasting events, unrest, and pre-eruptive activity can have on glacier velocity.

How to cite: Unnsteinsson, T., Spagnolo, M., Rea, B., Girona, T., Barr, I., and Mullan, D.: Feeling the heat: global detection of volcanic effects on glacier mass balance and dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14408, https://doi.org/10.5194/egusphere-egu26-14408, 2026.

EGU26-14679 | ECS | PICO | CR1.5

A proxy-based method of estimating glacier heat sources and transport mechanisms to map thermal processes at a regional scale 

Dia Martinez Gracey, Gwenn Flowers, and Mylène Jacquemart

Glacier thermal structure exerts a strong control on ice dynamics, yet it remains poorly characterized at the global scale. Despite its influence on glacier flow and, consequently, on melt and sea-level projections, thermal structure is typically neglected in large-scale glacier models. This omission stems from the fact that current methods of determining thermal structure require extensive field observations or computationally expensive modelling, resulting in only dozens of glaciers having well-defined thermal structures. In this work, we developed and applied a proxy-based approach to estimate the major heat sources (meltwater refreezing and strain heating) and transport mechanisms (advection and diffusion) in the heat transfer equation, which shapes glacier thermal structure. Proxies derived from publicly available observations and model output are calculated for glaciers in RGI-01 (Alaska) and RGI-07 (Svalbard and Jan Mayen). This framework enables a rapid regional assessment of thermal characteristics without requiring coupled thermomechanical modelling.

Across both Alaska and Svalbard, meltwater refreezing is the dominant heat source for 73% of glaciers, while diffusion dominates heat transport for 75% of glaciers. Note that this model only considers refreezing in the accumulation area, and 21% of these glaciers do not have an accumulation area. The majority (76%) of glaciers exhibit warmer accumulation-area ice transported toward cooler ablation areas. When examined by proxy rank, the most common pattern (47% of glaciers) is characterized by refreezing as the dominant heat source over strain heating, and vertical diffusion over horizontal advection as the primary transport mechanism. This pattern represents 25% of glacierized area, corresponding primarily to smaller glaciers (<10 km) scattered across Alaska, but found across sizes in Svalbard. Large Alaskan glaciers (39% of glacierized area), have a proxy pattern where refreezing dominates strong strain heating, while horizontal advection exceeds vertical diffusion. In Svalbard, this pattern is almost absent (<1% of glaciers). Comparing the proxy rank patterns of all glaciers in Alaska and Svalbard with those of glaciers with known thermal structures provides a correlation-based interpretation of the proxy results. For example, we found that the calculated proxy pattern for known temperate glaciers is characterized by dominant refreezing and advection, whereas known cold glaciers exhibit the pattern characterized by dominant refreezing over strain heating and diffusion over advection. Furthermore, a number of large glaciers on the continental side of the St. Elias Mountains in Alaska exhibit a proxy pattern distinct from those associated with well-established thermal structures in the region.

This work presents a way to calculate heat-source and transport-mechanism proxies as a practical means of estimating glacier thermal characteristics for any RGI region with sufficient input data. The resulting proxy distributions provide new insight into spatial patterns of heat generation and transfer in glaciers at the regional scale and establish a baseline for evaluating thermal responses to climate change. Moreover, these results can serve as comparative datasets for emerging emulator-based, regional-scale thermal modelling.

How to cite: Martinez Gracey, D., Flowers, G., and Jacquemart, M.: A proxy-based method of estimating glacier heat sources and transport mechanisms to map thermal processes at a regional scale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14679, https://doi.org/10.5194/egusphere-egu26-14679, 2026.

EGU26-15350 | ECS | PICO | CR1.5

Unveiling the subglacial landscape in the Southern Andes shows an abundance of future glacial lakes 

Jorge Andrés Berkhoff, David Farías-Barahona, Pablo Iribarren-Anacona, Christian Sommer, Marius Schaefer, José Luis Rodriguez, José Uribe, and Johannes J Fürst

Glaciers in the southern Andes are retreating rapidly because of ongoing climate warming. This process is reshaping the mountainous landscape and promoting the formation of new glacial lakes. Therefore, quantifying glacier ice thickness and subglacial topography is vitally important for assessing future water resources and glacier-retreat hazard. Of particular interest are bed over-deepening that will fill with water once they become ice-free. Such water bodies are potentially trigger sites for devasting Glacial Lake Outburst Floods (GLOF). However, estimates of ice thickness at the regional scale in the southern Andes remain uncertain due to the scarcity of in situ data on current glacier thickness as well as strong climatic and topographic gradients.

Here, we present a regional reconstruction of glacier ice thickness and subglacial topography for the entire Southern Andes, systematically constrained by the extensive archive of ground-penetrating radar measurements available for the region. Ice thickness is reconstructed, assuming perfect plasticity. Apart from direct measurements, we use glacier retreat and observe elevation changes to constrain the reconstruction. The resultant thickness map shows latitudinal contrasts in glacier geometry, with thin ice bodies in the desert Andes and substantially thicker ice masses in Patagonia.

We estimate a total volume of glacial ice of 5,960.6 km³ in the Southern Andes, equivalent to a global sea-level rise of 15.1 mm, with more than 95% of this volume concentrated in Patagonia, particularly in the two vast icefields there. By removing the modeled ice cover, we determine the subglacial topography and identify more than 6,000 overdeepenings that represent potential sites for future glacial lake formation. For each potential lake, we estimate its area, depth, and volume, yielding a total potential lake volume of approximately 177.6 km³ across the Southern Andes, with most of this volume concentrated in Patagonia (171.18 km³).

Our results provide a new measurement-informed, database for assessing future glacier evolution, freshwater storage, and emerging GLOF hazards in the Andes, providing critical information for climate adaptation and risk management in high-mountain regions

How to cite: Berkhoff, J. A., Farías-Barahona, D., Iribarren-Anacona, P., Sommer, C., Schaefer, M., Rodriguez, J. L., Uribe, J., and Fürst, J. J.: Unveiling the subglacial landscape in the Southern Andes shows an abundance of future glacial lakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15350, https://doi.org/10.5194/egusphere-egu26-15350, 2026.

EGU26-18021 | ECS | PICO | CR1.5

Alpine glacier response to increasing temperature between 2009 and 2022. Insights from photogrammetric analysis in the Ötztal and Zillertal Alps (AT). 

Natalie Barbosa, Christoph Mayer, Juilson Jubanski, Ulrich Münzer, Florian Siegert, and Michael Krautblatter

The European Alps have experienced massive glacier loss over the last decade, and 50% of all glaciers are expected to disappear even under current climate conditions by 2050. Glacier retreat, rapid meltwater production and damming, debustressing, and accelerated release of sediment massively increase the natural hazards in the region. The decline of glaciated areas in alpine regions directly impacts water reservoirs, tourist infrastructure, and alpine communities; therefore, precise quantification of rates of glacier retreat at a regional scale are paramount for foreseen prevention and mitigation plans.

The location and extent of mountain glaciers are conditioned by two independent factors: topography and climatic conditions. In this contribution, we explore the glacier changes over the last decade in two contrasting regions: (i) the drier and colder Ötztal Alps, host of the largest glaciers in Austria, and (ii) the wetter/warmer Zillertal Alps. Our aim is to decipher the key factors controlling glacier retreat at the regional scale. We used photogrammetric reconstruction of high-resolution aerial imagery at a 20cm resolution to (i) manually map the glacier extent in 2009/2010 and 2022 for 87 glaciers in the Zillertal and 48 glaciers in the Ötztal. The manual mapping was supported by stereographic visualizations for a precise photo-interpretation of glacier boundaries, (ii) quantify glacier retreat for each glacier in terms of relative area change (km2) and geodetic mass balance (m w.e.a-1), and (iii) calculate morphometric parameters such as slope and slope orientation. Finally, we contrasted ERA5 precipitation and temperature data with the findings.

This study presents a unique compilation of glacier extents and geodetic mass balance over 202 km² of the Ötztal and 184 km² of the Zillertal Alps from 2009 to 2022. Despite the contrasting morphological and climatic characteristics, glaciers in both mountain ranges retreat at similar rates. These findings demonstrate the dominant climatic control on glacier loss in the Eastern Alps and suggest that, under current climatic conditions, glacier morphology plays a minor role at the regional scale. 

How to cite: Barbosa, N., Mayer, C., Jubanski, J., Münzer, U., Siegert, F., and Krautblatter, M.: Alpine glacier response to increasing temperature between 2009 and 2022. Insights from photogrammetric analysis in the Ötztal and Zillertal Alps (AT)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18021, https://doi.org/10.5194/egusphere-egu26-18021, 2026.

EGU26-20051 | ECS | PICO | CR1.5

Glacier mass balance modeling using a Long Short-Term Memory network 

Marijn van der Meer, Harry Zekollari, Alban Gossard, Kamilla Hauknes Sjursen, Jordi Bolibar, Matthias Huss, and Daniel Farinotti

Glacier mass balance is a key indicator of climate change and a central driver of glacier evolution, yet most glaciers worldwide lack long-term in-situ measurements. For estimating glacier mass balance, data-driven models offer a complementary pathway to traditional numerical approaches by learning empirical relationships between climate forcing, topography, and mass balance directly from observations. Here, we develop a recurrent neural network based on a Long Short-Term Memory (LSTM) architecture within the Mass Balance Machine (MBM) framework and evaluate its ability to predict seasonal and annual point surface mass balance across the Swiss Alps. MBM is trained on 30'000 point observations from 30 glaciers and tested on eight glaciers excluded from training to assess spatial generalization. MBM predicts both winter and annual mass balance with high accuracy on unseen glaciers, and its recurrent structure provides a clear advantage by allowing the model to learn temporal dependencies, which improves the representation of seasons with strong accumulation or ablation. Beyond point predictions, MBM produces spatially distributed mass balance maps that closely resemble reference products directly derived from in-situ data, capture elevation-dependent gradients, and yield glacier-wide mass changes consistent with the differencing of repeated terrain models. Monthly outputs further show that the model captures the seasonal transition from winter accumulation to summer ablation and its dependence on elevation with realistic timing and magnitude. These results indicate that a recurrent neural network approach can recover key characteristics of glacier mass balance dynamics from sparse in-situ observations and that the learned relationships are transferable across glaciers with distinct meteorological and topographic settings. The demonstrated generalization skill and suitability for transfer learning highlight the potential of MBM for predicting glacier mass balance in regions with limited or no direct measurements.

How to cite: van der Meer, M., Zekollari, H., Gossard, A., Hauknes Sjursen, K., Bolibar, J., Huss, M., and Farinotti, D.: Glacier mass balance modeling using a Long Short-Term Memory network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20051, https://doi.org/10.5194/egusphere-egu26-20051, 2026.

EGU26-2219 | ECS | PICO | HS6.1

Temporal Variability and Trend Analysis of Monthly Snow Cover in a Himalayan river basin 

Harshita Tiwari, Aditya Kumar Thakur, and Rahul Dev Garg

Snow cover variability in high-altitude Himalayan river basins plays a critical role in regulating regional hydrology, water availability, and climate-cryosphere interactions. Understanding its temporal behaviour is particularly important for snow-fed basins such as the Budhi Gandaki Basin, Nepal, where seasonal meltwater significantly influences downstream flow regimes. Previous studies often overlooked detailed monthly-scale time series analysis and robust trend diagnostics of snow cover variability. In this study, we investigate the temporal dynamics of monthly snow cover area in the Budhi Gandaki Basin (area: 3857.85 km²) using continuous observations from 2020 to 2024 using the Moderate Resolution Imaging Spectroradiometer (MODIS) 8-day snow cover products (MOD10A2) with 500 m resolution. A comprehensive time-series framework was applied, incorporating descriptive statistics, linear trend analysis, seasonal climatology, anomaly assessment, and non-parametric trend detection. The MOD10A2 snow cover composites were spatially averaged over the basin and temporally aggregated to monthly resolution using a proportional day-overlap weighting scheme to estimate basin-averaged monthly snow covered area (SCA). Monthly snow cover data were then transformed into a continuous time series to evaluate overall variability and long-term behaviour. Seasonal characteristics were quantified through monthly climatology and interannual variability using mean and standard deviation metrics. Trend significance was examined using the Mann-Kendall test, while the magnitude of change was estimated using Sen’s slope. Results reveal a mean snow cover index of 0.56 with substantial variability showing a standard deviation of 0.16 snow cover fraction (SCF), indicating pronounced seasonal and interannual fluctuations. Monthly climatology shows maximum snow cover during winter months, peaking in February (mean: 0.762 SCF) and January (mean: 0.756 SCF), while minimum values occur during the summer monsoon period, particularly in July (mean: 0.424 SCF) and June (mean: 0.426 SCF). Linear trend analysis indicates a gradual declining tendency in snow cover at a rate of -0.0024 SCF per month. However, the Mann-Kendall test yields a Z statistic of -1.77 with a p-value of 0.076, suggesting that the observed decreasing trend is not statistically significant at the 95% confidence level. Anomaly analysis further highlights episodic deviations from the climatological mean, with maximum positive and negative anomalies of +0.204 SCF and -0.162 SCF, respectively, reflecting short-term climate-driven variability. Overall, the findings indicate a weak but persistent declining tendency in snow cover, modulated strongly by seasonal and interannual variability rather than a statistically significant long-term trend. This study provides an improved understanding of snow cover dynamics in the Budhi Gandaki Basin and offers valuable insights for hydrological modeling, climate impact assessments, and sustainable water resource management in snow-fed Himalayan river systems.

Keywords: Snow cover variability; Time series analysis; Himalayan river basin; Seasonal climatology; Trend detection

 

How to cite: Tiwari, H., Thakur, A. K., and Garg, R. D.: Temporal Variability and Trend Analysis of Monthly Snow Cover in a Himalayan river basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2219, https://doi.org/10.5194/egusphere-egu26-2219, 2026.

Seasonal snow cover in high mountain regions plays an important role in river flow hydrographs, water availability and land atmosphere interactions. In the Western Himalaya, mapping snow cover accurately is difficult due to frequent cloud cover, steep terrain, strong shadow effects and confusion between snow, clouds and bright rocky surfaces in satellite images. The study shows that these issues are clearly observed in the Western Himalayas, where the lack of sufficient ground reference data further limits the use of fully supervised classification methods. To address these challenges, the objective of the present study is to develop a snow cover mapping framework that leverages self-supervised learning for robust feature representation from satellite remote sensing data in the Western Himalaya. The method focuses on learning useful snow related features directly from large volumes of unlabelled satellite images, reducing the need for extensive manually labelled training data. Multi temporal optical satellite images are used so that the model can learn stable snow patterns across different seasons, illumination conditions and surface states. A convolutional neural network is trained using a contrastive self-supervised learning strategy, where different augmented versions of the same image patch are treated as similar samples, while patches from different locations are treated as dissimilar. The self-supervised encoder is coupled with a lightweight decoder in an encoder-decoder segmentation architecture, enabling pixel wise snow mapping while preserving spatial detail under limited supervision. Simple data augmentations, such as brightness changes, contrast adjustments and random cropping are applied to improve the model’s ability to recognize snow under varying conditions while preserving its key spectral and spatial characteristics. After self-supervised pretraining, the learned feature representations are fine tuned for snow and non-snow classification using a limited set of labelled samples derived from reference snow products and manual interpretation. This greatly reduces the dependence on large labelled datasets compared to conventional supervised learning methods. Snow cover maps are generated for different seasons and elevation zones to examine spatial and temporal variability of snow distribution across the basin. The results are compared with traditional index based methods, such as Normalized Difference Snow Index (NDSI) thresholding, especially in areas affected by clouds, shadows and mixed land cover. The study shows that the self-supervised learning provides a practical and reliable framework for snow cover mapping in data scarce and high altitude regions. The methodological framework developed in this study can be utilized for other basins also to have improved understanding of snow cover dynamics.

Keywords: Snow cover; self-supervised learning; remote sensing; Himalaya

How to cite: Thakur, V., Keshari, A. K., and Tak, S.: Monitoring of Spatio-Temporal Snow Cover using AI Based Self-Supervised Learning in Data Scarce Himalayan River Catchment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3445, https://doi.org/10.5194/egusphere-egu26-3445, 2026.

Water management represents a critical challenge for the mining industry, as large volumes of surface water must be controlled and treated during operations to ensure the stability of geotechnical structures and protect the environment. This extends beyond the operational phase, as it is essential to ensure the physical stability of tailings storage facilities and to limit the potential transport of contaminants on reclaimed mine sites. The water balance of tailings storage facilities is regulated by surface water management and often treatment infrastructures. In addition, the water balance is also closely linked to the performance of several engineered cover systems used to reclaim tailings storage facilities. Because tailings storage facilities generally occupy large areas, snow accumulation in winter and rapid melting in spring generate substantial volumes of meltwater within a short period. Thus, the spring freshet is a critical phase for water inventory control, from operation to post-reclamation. In this context, developing tailored monitoring tools is essential to ensure effective spring water management on tailings storage facilities.

This work aims to develop a high spatial resolution drone-based sensing approach for semi-real-time monitoring of the snow water balance in tailings storage facilities during snowmelt. This study is based on the results of several drone-based Structure-from-Motion photogrammetry and LiDAR surveys conducted during snowmelt on a reclaimed tailings storage facility. The site presents two major challenges for these sensing techniques: a flat, featureless area prone to oversaturated whites when covered with snow, and sections of dense low vegetation that reduce LiDAR signal penetration and hinder the generation of accurate digital elevation models. The accuracy and precision of the two remote sensing technologies to evaluate the snow depth were assessed based on manual measurements and conventional GNSS surveys. The impact of the reconstruction software/algorithms and parameters, as well as the number of ground control points (between 3 and 21) used in the reconstructions, on accuracy was also assessed. Finally, a preliminary snow-water equivalent model was developed and integrated within the data processing scheme to provide the changes of snow-water equivalent during snowmelt. Results show that LiDAR is the most accurate and reliable approach to monitor the snow depth. Photogrammetry-derived digital elevation models resulted in an error up to 66 cm. The quality and accuracy of photogrammetric surveys depend on the number of ground control points, the reconstruction algorithm used, and the absence of aerotriangulation tie points in certain areas. A snow-water equivalent model was integrated with LiDAR-derived snow depth data to characterize the temporal evolution of the tailings storage facility water balance during snowmelt. This presents an incremental improvement towards effective spring-water management on tailings storage facilities.

How to cite: Boulanger-Martel, V. and Blatter, N.: Potential of LiDAR and Structure-from-Motion Photogrammetry for High-Resolution Monitoring of Snowmelt Water Balance in Tailings Storage Facilities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8352, https://doi.org/10.5194/egusphere-egu26-8352, 2026.

EGU26-8577 | PICO | HS6.1

Updates on advancements of the Terrestrial Snow Mass Mission 

Benoit Montpetit, Chris Derksen, Vincent Vionnet, Marco Carrera, Julien Meloche, Nicolas Leroux, and Jean Bergeron

Snow is the only component of the water cycle that does not have a dedicated earth observation mission. Snow impacts many sectors like the health and well-being of communities, the economy, and sustains ecosystems. Snow also contributes to many costly hazards like floods, droughts, and avalanches. The current lack of information on how much water is stored as snow (snow water equivalent, SWE), and how it varies in space and time, limits the hydrological, climate, and weather services provided by Environment and Climate Change Canada (ECCC). To address this knowledge gap, ECCC, the Canadian Space Agency (CSA) and Natural Resources Canada (NRCan) are working in partnership to advance the scientific and technical readiness for a Ku-band synthetic aperture radar (SAR) mission presently named the ‘Terrestrial Snow Mass Mission’ – TSMM. An observing concept capable of providing dual-polarization (VV/VH), moderate resolution (500 m), wide swath (~250 km), and high duty cycle (~25% SAR-on time) Ku-band radar measurements at two frequencies (13.5; 17.25 GHz) is under development. This Canadian radar mission will provide weekly coverage of the northern hemisphere with Ku-band SAR data, and coupled with modeled data in the Canadian Land Data Assimilation System (CaLDAS), will provide daily snow water equivalent data, to assist hydrological applications and decision-making. It has been proven that Ku-Band backscatter measurements are sensitive to SWE through the volume scattering of the signal by the snow microstructure. Radar measurements are also well known to be able to discriminate between wet and dry snow conditions.

In this presentation, we will review recent progress at ECCC (supported by the mission science team and the international snow community). Key areas of ongoing development include:
(1) The Ku-band radar SWE retrieval algorithm proof of concept, based on the use of physical snow modeling to provide initial estimates of snow microstructure which can effectively parameterize forward model simulations for prediction of snow volume scattering.
(2) Improvements to radiative transfer modelling codes to improve computation efficiency.
(3) Improvements to physical snow modeling in the Canadian land surface model Soil Vegetation Snow version 2 (SVS2).
(4) Development of the capability for direct assimilation of Ku-band backscatter into environmental prediction systems at ECCC.
(5) Segmentation of wet from dry snow based on the time evolution of radar backscatter.

Testbed experiments in which snow physical modeling, SWE retrievals, and data assimilation are analyzed collectively are currently under development. These experiments will be facilitated by the TSMM simulator and will incorporate outputs from SVS2 and are supported by airborne and ground-based Ku-band radar measurements from national and international academic partners. 

How to cite: Montpetit, B., Derksen, C., Vionnet, V., Carrera, M., Meloche, J., Leroux, N., and Bergeron, J.: Updates on advancements of the Terrestrial Snow Mass Mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8577, https://doi.org/10.5194/egusphere-egu26-8577, 2026.

Abstract: Snow is a critical component of the cryosphere, exhibiting substantial variations in both spatial and temporal dimensions. Accurately capturing the dynamic characteristics of seasonal snow cover is essential for predicting snowmelt runoff, monitoring hydrological cycle, and conducting climate change analysis. Optical satellite remote sensing has proven to be an effective tool for monitoring global and regional snow cover. However, existing fractional snow cover (FSC) data derived from optical imagery often encounters challenges, including large-scale spatial gaps caused by cloud cover and shadows. Meanwhile, passive microwave data, although valuable, typically possess lower spatial resolution, rendering them inadequate for detecting snow cover dynamics under complex surface conditions. In this study, we employed a fractional snow cover fusion estimation method to generate high-resolution (1 km) spatiotemporally continuous FSC estimation datasets for the Tibetan Plateau region from the years 2008 to 2021, regardless of weather conditions. The accuracy of the FSC data was systematically evaluated over the study period, demonstrating excellent consistency with independent datasets, including Landsat-derived FSC (total 20 scenes; RMSE = 0.092–0.193; R = 0.83–0.946) and ground-based snow observations (Approximately 70,000 site records; Overall Accuracy = 0.95; Kappa = 0.95). Furthermore, the FSC datasets produced by this method exhibits superior performance in accurately capturing the complex daily snow cover dynamics compared to other FSC datasets(Overall Accuracy: 0.95 vs. 0.91 vs. 0.85). In conclusion, the daily FSC maps of the Tibetan Plateau generated from 2008 to 2021 using data fusion methods in this study offer high accuracy and complete spatiotemporal coverage. These FSC datasets hold substantial value for climate projections, hydrological studies, and water management at both global and regional scales.

Fig.1 Spatial Distribution of Snow Cover (1 km) for daily FSC data over the Tibetan Plateau from 2008 to 2021. The dates are shown at the bottom of the subplots. The blank areas denote missing values due to various reasons. The range of snow cover variation is from 0 to 1, where 0 indicates no snow cover and 1 indicates full snow cover.

Table.1 Summary of accuracy metrics for the 1km daily fractional snow cover data over the Tibetan Plateau using 10 Landsat scenes FSC data as the reference data.

How to cite: Sun, T. and He, T.: Mapping 1 km Fractional Snow Cover from Passive Microwave Brightness Temperature Data and MODIS Snow Cover Product over The Tibetan Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10752, https://doi.org/10.5194/egusphere-egu26-10752, 2026.

EGU26-10848 | ECS | PICO | HS6.1

Machine Learning–Based Gap-Filling of Satellite Snow Products Using Time-Lapse Photography and Meteorological Data 

Ján Krempaský, Veronika Lukasová, Ivan Mrekaj, Milan Onderka, and Svetlana Varšová

Reliable information on snow cover dynamics is essential for water resource management, climate impact assessments, and ecological studies. In mountainous regions, where spatial variability is high and long-term observations are limited, satellite-based snow products often present the primary source of information. However, their performance is constrained in complex terrain by cloud cover, coarse spatial resolution, and data gaps. Therefore, the validation of satellite-derived snow cover data is crucial for reducing uncertainty. In this study, we employed a low-cost, ground-based time-lapse camera to monitor snow cover (SC) and to support the validation, gap-filling, and improved reliability of satellite-derived snow cover products.

Time-lapse photography was obtained using a camera trap installed at the Skalnaté Pleso Observatory in the High Tatra Mountains (Slovakia). The camera captured daily images of a south-eastern slope during four snow seasons (2021/22–2024/25). An automated image-processing workflow was applied to derive snow cover percentage from the photographs, including horizon-based image alignment, masking of non-relevant areas, and automatic snow classification based on blue-band intensity thresholds. The resulting camera-derived SC was compared with satellite-based fractional snow cover (FSC) from Sentinel-2 products (Fractional Snow Cover and Gap-filled Fractional Snow Cover marked as S_FSC and S_GFSC) and MODIS products (MOD10 and MYD10 marked as M_TERRA_FSC and M_AQUA_FSC) within the camera’s field of view.

The analysis revealed substantial differences in data availability between ground-based and satellite observations, with time-lapse photography providing more continuous records during periods of frequent cloud cover. Camera-derived SC captured short-term snow accumulation and melt dynamics that were often missed or temporally smoothed in satellite products. Relative to camera observations, Sentinel products overestimated SC by 11.3 % (S_GFSC) and 9.1 % (S_FSC), whereas MODIS products underestimated SC by -9.5 % (M_AQUA_FSC) and -7.7 % (M_TERRA_FSC). 

Data gaps in satellite products were addressed using a Random Forest machine-learning approach trained on SC derived from terrestrial time-lapse photography. To avoid sensor-mixing biases, separate models were trained for each Sentinel-2 and MODIS product. By integrating local meteorological variables such as daily air temperature, precipitation, snow depth, and global radiation, the models were able to capture the non-linear nature of snow dynamics. Our study demonstrates that combining time-lapse photography with satellite products and in situ meteorological measurements enables more accurate reconstruction of snow cover dynamics, particularly in periods of rapid snow accumulation and melt in alpine environments.

Acknowledgement: This study was funded by the project VEGA 2/0048/25.

How to cite: Krempaský, J., Lukasová, V., Mrekaj, I., Onderka, M., and Varšová, S.: Machine Learning–Based Gap-Filling of Satellite Snow Products Using Time-Lapse Photography and Meteorological Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10848, https://doi.org/10.5194/egusphere-egu26-10848, 2026.

EGU26-12080 | ECS | PICO | HS6.1

Measuring mine dust contamination of snow in northern Sweden using optical remote sensing 

Moon Taveirne, Christian Zdanowicz, Alexandre Langlois, Biagio Di Mauro, Giacomo Traversa, and Axel Hagermann

Mineral dust is produced as a by-product when mining for metals such as iron and rare-earth elements. Around mines in the Arctic and Subarctic, this dust is transported by wind and deposited on the snow surface, contaminating the seasonal snowpack. The presence of mine dust darkens the snow surface, resulting in a lower snowpack albedo. Due to their lowered albedo, seasonal snowpacks that contain mine dust experience accelerated melting. Nordic countries, including Sweden, are showing an increasing interest in the expansion of mining activities due to increasing demand for metals to use in technology and a desire to produce raw materials within Europe. The Kirunavaara mine in the Swedish Arctic is Europe’s largest iron mine, and is an accordingly large source of mineral dust, which spreads around the adjacent town of Kiruna and the surrounding areas.

One possible approach to quantify mine dust contamination of the seasonal snowpack is using optical remote sensing. The change in spectral reflectance of the contaminated snow surface is used to infer optical properties and the concentration of mine dust in the surface snow. Spectral indices and radiative transfer modelling are applied to the spectral reflectance data to retrieve dust concentrations. We have measured dust concentrations in snow around Kiruna during spring 2025, and measured reflectance of the affected snow surfaces. Snow darkening in Kiruna occurs predominantly in the area located downwind from the mine where dust concentrations in snow are highest. Dust loadings in surface snow around Kiruna reach over 2000ppm, with associated snow broadband albedo values as low as 0.3 in the most heavily contaminated areas. There is a clear relationship between broadband albedo and mine dust concentrations in the surface snow. However, the spectral signatures of the contaminated snow surface show that iron mine dust darkens the snow relatively evenly across all wavelengths of visible light. Combined with the high dust loading, this even darkening effect means that previously established spectral indices for minerals dust in snow are not applicable in the case of iron dust contamination, and an approach tailored specifically to this type of dust is required.

How to cite: Taveirne, M., Zdanowicz, C., Langlois, A., Di Mauro, B., Traversa, G., and Hagermann, A.: Measuring mine dust contamination of snow in northern Sweden using optical remote sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12080, https://doi.org/10.5194/egusphere-egu26-12080, 2026.

EGU26-12971 | PICO | HS6.1

Development of an Advanced L2 Processor for PRISMA Second-Generation within the COOL Project: Application to Snow-Covered Terrain 

Federico Santini, Angelo Palombo, Saham Mirzaei, Stefano Pignatti, and Simone Pascucci

The COOL project, funded by the Italian Space Agency (ASI), focuses on the development of an advanced, modular Level-2 (L2) processor for the PRISMA Second-Generation (PRISMA-SG) hyperspectral mission. The processor is designed to generate high-quality L2 products, including surface reflectance, water vapor content, and aerosol optical thickness, while addressing the unique challenges introduced by the off-nadir acquisition geometry of the PRISMA-SG sensor.

The processor builds upon state-of-the-art radiative transfer modeling and integrates physics-based atmospheric and topographic correction algorithms based on the MODTRAN6 model. The processing chain is derived and extended from previous work (Santini & Palombo, 2019; Palombo & Santini, 2020; Santini & Palombo, 2022), and incorporates second-order effects, such as adjacency corrections and topographic illumination variations. These algorithms are carefully adapted to the spectral, spatial, and viewing geometry characteristics of PRISMA-SG, aiming to achieve or exceed a Scientific Readiness Level (SRL) of 6.

Validation of the processor relies on both simulated datasets and in-situ measurements over dedicated calibration and validation (CAL/VAL) sites established within the COOL project. Top-of-atmosphere (TOA) radiance signals are simulated over these sites and compared with field measurements to quantify residual errors and assess the sensitivity of the inversion algorithms to off-nadir acquisition effects. These activities ensure the robustness and scientific usability of the derived L2 products in both nadir and off-nadir observation modes.

As a demonstration, the L2 processor was applied to PRISMA-SG images acquired over snow-covered areas in the Italian Alps. The results were compared with the standard L2 products provided by the image supplier. The comparison shows close general agreement in reflectance spectra while correcting artifacts present in the standard products, including topographic effects, adjacency effects, and off-nadir-induced reflectance overestimation. Notably, the corrected reflectance values remain physically consistent and do not exceed unity, a problem often observed in the standard products.

This work consolidates the L2 processing capabilities for PRISMA-SG, providing validated, reliable, and application-ready hyperspectral products. The approach demonstrates the importance of accounting for off-nadir geometry and second-order atmospheric and topographic effects, enabling robust use of PRISMA-SG data for environmental monitoring, snow cover studies, and other Earth observation applications.

How to cite: Santini, F., Palombo, A., Mirzaei, S., Pignatti, S., and Pascucci, S.: Development of an Advanced L2 Processor for PRISMA Second-Generation within the COOL Project: Application to Snow-Covered Terrain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12971, https://doi.org/10.5194/egusphere-egu26-12971, 2026.

EGU26-17516 | PICO | HS6.1

Are snow patterns well modelled when simulating river discharge in Mediterranean mountain catchments? A multimodel approach assessment using remote sensing data 

Raquel Gómez-Beas, Marta Egüen, Giuseppe Formetta, María José Polo, and Rafael Pimentel

Modelling streamflow in mountainous areas is challenging. The presence of snow is an additional factor to consider, as it is the primary driver of streamflow dynamics in mountain catchments. In addition, this complexity increases in the Mediterranean mountains, where snow dynamics are more variable, with specific characteristics, including shallow snowpack, high density, and evaposublimation rates that cannot be neglected when assessing water resource availability during the dry season. Many approaches, with varying levels of complexity, have been used to model streamflow in mountainous areas. In general, these models are calibrated and evaluated against streamflow without considering their performance with respect to snow dynamics. That is, river discharges are well represented, but not due to the correct reasons.

This study assesses the implications of selecting snow parameterizations for streamflow modelling in Mediterranean mountain catchments, considering not only streamflow but also snow performance. Five different hydrological models, with different conceptualizations – lumped, semi-distributed, and fully distributed – and with different levels of complexity regarding snow parameterization – degree-day, radiation-day, and mass and energy balance approach– have been used. These models are: (1) GR4J associated with CemaNeige (lumped with degree-day snow model), (2) SWAT (semidistributed with degree-day snow model), (3) HYPE (semidistributed with radiation-day snow model), (4) GEOFRAME (semidistributed with temperature-radiation-day snow model), and (5) WiMMed (distributed with mass and energy balance snow model). Models were calibrated against streamflow observations and evaluated for snow performance using remote-sensing-derived snow-cover area. A spectral mixture analysis carried out using Landsat imagery, considering the three main land cover types over the region: snow, shallow vegetation, and rocks, was performed to define the fraction of snow in each cell. The values of these pixels were aggregated at the catchment scale for comparison with the simulations. The Guadalfeo River basin in southern Spain has been selected as representative of a Mediterranean mountain-coastal catchment for this analysis.

Preliminary results indicate that the complexity of snow dynamics is better captured by the more complex approach, namely, the fully distributed mass and energy balance snow model. However, the assessment indicates that simpler approaches can be valid when analyzing changes and seasonality rather than actual values. This observation underscores the potential to use this model in an ensemble to compute hydrological uncertainty, as is common in hydrological seasonal prediction and climate studies.

Acknowledgments: This work is part of the project PCI2024-153496, funded by MCIU/AEI/10.13039/501100011033 and EU

How to cite: Gómez-Beas, R., Egüen, M., Formetta, G., Polo, M. J., and Pimentel, R.: Are snow patterns well modelled when simulating river discharge in Mediterranean mountain catchments? A multimodel approach assessment using remote sensing data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17516, https://doi.org/10.5194/egusphere-egu26-17516, 2026.

EGU26-18431 | PICO | HS6.1

Evaluating the use of NRB Sentinel-1 product for reconstructing high resolution SWE in mountains 

Carlo Marin, Valentina Premier, Nikola Mang, and Davide Castelletti

Seasonal snow in mountain catchments is highly heterogeneous, yet snow water equivalent (SWE) is rarely available at spatial and temporal scales useful for hydrology and ecosystem applications. We present a multi-source retrospective SWE reconstruction framework that produces daily 30-meter resolution SWE over mountains by integrating (i) SAR-based wet-snow information from Sentinel-1 Normalised Radar Backscatter (NRB) product; (ii) optical snow-cover dynamics given using Sentinel-2 and Sentinel-3 data and (iii) in-situ meteorological forcing. A key advantage is that the method does not rely on spatially distributed precipitation fields, which remain a dominant uncertainty in mountain snow modelling.

The approach is built around a pixel “state” concept (accumulation, equilibrium, ablation) that constrains physically plausible SWE evolution through the season. Snow presence is represented by a daily high-resolution snow-cover-area (SCA) time series obtained by gap-filling and downscaling coarse snow-cover fraction with high-resolution optical observations, followed by a state-aware regularization that removes implausible transitions. Snow melt is computed using an enhanced temperature-index (ETI) model driven by air temperature and incoming shortwave radiation. However, ETI formulations do not explicitly resolve cold content and internal energy storage; as a result, they can trigger melt earlier than expected, as they do not account for delays imposed by the snowpack thermal inertia. To constrain the onset of true meltwater conditions, we integrate Sentinel-1 wet-snow maps derived from the new NRB time series, using multi-temporal backscatter changes to detect wet-snow conditions.

The Sentinel-1 NRB product provides radiometrically terrain-corrected backscatter (γ⁰) using the local incidence angle and mapping the data onto a reference coordinate system [1]. This improves consistency over complex topography compared to conventional Level-1 GRD processing. In addition, a novel cloud-native Zarr format enables fast, chunked access to long time series, facilitating regional-scale analyses.

We demonstrate the method in the Maipo region (Andes), where shortwave radiation dominates snowmelt. Preliminary results show that combining daily optical snow-cover dynamics with NRB-informed wet-snow timing enables SWE reconstructions that are temporally consistent across full seasons and, critically, prevents ETI-driven melt before liquid water is detected. Additionally, in the presentation, the NRB products and their assessment for the analysis of timeseries over mountains will be provided.

References

[1]  G. H. X. Shiroma, M. Lavalle and S. M. Buckley, "An Area-Based Projection Algorithm for SAR Radiometric Terrain Correction and Geocoding," in IEEE Transactions on Geoscience and Remote Sensing, vol. 60, pp. 1-23, 2022.

How to cite: Marin, C., Premier, V., Mang, N., and Castelletti, D.: Evaluating the use of NRB Sentinel-1 product for reconstructing high resolution SWE in mountains, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18431, https://doi.org/10.5194/egusphere-egu26-18431, 2026.

Mountain snow is a critical component of the hydrological cycle and climate system, making reliable information on snow depth (SD) essential for water resource management and climate studies. Estimating SD in mountainous terrain remains challenging due to complex topography, heterogeneous land cover, and highly variable snow and weather conditions. Synthetic Aperture Radar (SAR) is suitable in such environments, as it provides frequent observations, high spatial resolution, and sensitivity to snow properties independent of cloud cover and illumination. In particular, Sentinel-1 C-band SAR backscatter-based method enables large-scale and continuous SD monitoring, but faces limitations in vegetated, shallow, or wet snow conditions. To overcome these limitations, this study proposes an improved machine learning (ML) framework that incorporates new input variables derived from Sentinel-1 and other optical data, improving upon existing Sentinel-1–based ML approaches for SD estimation. Additionally, the framework is designed for efficient implementation using preprocessed Sentinel-1 data available in Google Earth Engine, thereby minimising the computational burden of handling SAR data and facilitating scalable application across regions and time periods. The methodology is implemented across three climatically and physiographically distinct mountainous regions: the Colorado Rocky Mountains, the European Alps, and the Indian Western Himalayas. Across all three regions, the proposed model substantially performs better than the existing methods, achieving MAE(r) values of 7.9 cm (0.96), 22.3 cm (0.91), and 68.4 cm (0.72), respectively. Since the physical scattering processes governing C-band SAR responses to snow are not yet fully characterized, explainable AI techniques are applied to interpret model predictions and quantify the influence of input variables under varying environmental conditions. The results show region-specific and seasonal dependencies linked to snow type, vegetation cover, and surface conditions, providing new physical insights into the sensitivity of Sentinel-1 C-band backscatter to snow depth.

How to cite: Rajendiran, C. P. and Ramsankaran, R.: Physical Insights into Sentinel-1 SAR-Based Snow Depth Estimation Using Machine Learning and Explainable AI Across Different Mountainous Regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19246, https://doi.org/10.5194/egusphere-egu26-19246, 2026.

EGU26-19704 | ECS | PICO | HS6.1

Estimating daily high-resolution snow cover in the Central Pyrenees using logistic regression with Sentinel-2 and MODIS data 

Martí Navarro Planes, Xavier Pons, and Lluís Gómez Gener

The presence or absence of snow in the landscape strongly modulates land surface energy exchanges and governs key ecosystem processes in high-mountain catchments. In mid-latitude mountain regions, such as the Pyrenees, which are dominated by intermittent and ephemeral seasonal snowpacks, pronounced intra-annual spatial variability in snow cover complicates the accurate characterisation of snow temporal dynamics.

Although a wide range of snow products and remote sensing platforms are currently available, many of them have significant limitations when applied to complex, mountainous environments such as the Pyrenees. These limitations include data gaps caused by cloud cover and confusion between snow and clouds; reduced accuracy in areas affected by topographic shadows; insufficient illumination due to low solar elevation at the time of satellite overpass; and the trade-off between spatial and temporal resolution. Furthermore, as most existing products are designed for large-scale applications, they can introduce significant errors when high spatial detail is required. This is particularly pertinent in catchment- and sub-catchment-scale hydrological, biogeochemical, and ecological studies.

In this context, we propose a methodological approach that combines the daily temporal resolution of snow gap-filled MODIS products with Sentinel-2-derived snow cover as the ground truth, using k-nearest neighbour (k-NN) classification. We generated daily binary snow presence/absence maps at a spatial resolution of 20 m over the study area using a logistic regression model incorporating general explanatory variables such as elevation, slope, aspect, monthly solar radiation and the spatial and temporal information of snow cover, such as distance-to-snow maps derived from MODIS.

Preliminary results show that the logistic regression framework generates daily snow cover maps that are spatially and temporally consistent, substantially reducing data gaps and improving the representation of intermittent and ephemeral snow zones, which are expected to become increasingly prevalent under future climate change. Model outputs were evaluated against independent ground-based observations, including snow pole measurements, telenivometer data, showing good agreement across elevation gradients and seasons. Together, these results demonstrate the potential of the proposed approach to capture fine-scale spatio-temporal variability in snow cover, providing a robust basis for catchment-scale analyses of snow–hydrology and snow–biogeochemistry interactions in high-mountain regions.

How to cite: Navarro Planes, M., Pons, X., and Gómez Gener, L.: Estimating daily high-resolution snow cover in the Central Pyrenees using logistic regression with Sentinel-2 and MODIS data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19704, https://doi.org/10.5194/egusphere-egu26-19704, 2026.

EGU26-20414 | PICO | HS6.1

Evaluating uncertainties in modeled snow reflectance using UAV-based hyperspectral imaging and multispectral remote sensing 

Eric A Sproles, Dulio Fonseca-Gallardo, Shannon Hamp, Joseph A Shaw, Jeremy Wood, Henna-Retta Hanula, Roberta Pirazzini, and Riley D Logan

Snow albedo is a key control on surface energy balance in snow-covered environments, yet its estimation from multispectral satellite observations remains uncertain due to limited spectral resolution and spatial heterogeneity in snow reflectance. Thus, accurate surface albedo estimates over snow-covered landscapes are critical for the development of reliable satellite-based albedo products. However, validation data in snowy environments remains scarce, especially at high spatial resolution. This is problematic because within a single satellite scene, snow surfaces often exhibit substantial variability that challenges assumptions of spectral homogeneity of snowpack underlying many reflectance-to-albedo parameterizations.


We present a comparative framework that integrates hyperspectral Unmanned Aerial Vehicle (UAV) observations with multispectral satellite data to evaluate the limitations of derived snow albedo within the spectral configurations of Landsat 8, Landsat 9, and Sentinel 2. Our assessment extended across three distinct snowscapes: alpine, prairie, and taiga in Montana (USA), Montana, and Northern Finland; respectively. Our field-based approach employed two commercial hyperspectral sensors (Resonon Pika L and IR-L), to measure surface reflectance across the VIS–NIR–SWIR range (400-1700 nm; Landsat Bands 1-6; Sentinel 2 Bands 1-11) at high spectral (>250 bands) and spatial (0.3 m) resolution.


We isolated snow-only satellite scenes using a Convolutional Neural Network, enabling the identification of heterogeneous snow surfaces within each snowscape. Hyperspectral reflectance measurements were transformed into Landsat- and Sentinel-equivalent band reflectance using weighted sensor response functions, enabling direct band-wise comparison between hyperspectral and multispectral observations.


Our results highlight systematic discrepancies in Landsat reflectance: notably, strong overestimations in Bands 1, 2, and 5, and a consistent underestimation in Band 6 (SWIR1), with surface reflectance biases reaching up to 17%. The CNN-based classification highlighted the high spatial variability in snow reflectance, underscoring the limitations of assuming homogeneous conditions. These findings demonstrate the need to enhance validation strategies for snow-covered regions and provide a scalable protocol that integrates UAV-based acquisitions, high-resolution spectral measurements, and supervised scene analysis. This work contributes to improved characterization of snow albedo uncertainty and supports refinement of satellite-derived snow albedo products for cryospheric applications.

How to cite: Sproles, E. A., Fonseca-Gallardo, D., Hamp, S., Shaw, J. A., Wood, J., Hanula, H.-R., Pirazzini, R., and Logan, R. D.: Evaluating uncertainties in modeled snow reflectance using UAV-based hyperspectral imaging and multispectral remote sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20414, https://doi.org/10.5194/egusphere-egu26-20414, 2026.

EGU26-20729 | ECS | PICO | HS6.1

Snow Water Equivalent retrieval and InSAR Coherence modeling using L-band Lutan-1 data 

Jingtian Zhou, Yang Lei, Jinmei Pan, Weiliang Li, and Jiancheng Shi

Snow Water Equivalent (SWE) is a critical parameter in the global and regional water cycle and climate system. However, accurately measuring SWE change using satellite remote sensing remains a challenge. While the Interferometric Synthetic Aperture Radar (InSAR) is a promising technique to retrieve SWE from space, its application has been constrained until recently by the lack of spaceborne observations combining optimal low-frequency (e.g., L-band) radar frequencies with short temporal baselines. Furthermore, interferometric coherence is a key factor that affects the accuracy of the unwrapped phase and the subsequent SWE retrieval. However, the repeat-pass InSAR coherence modelling over snow has not been sufficiently investigated.

Our study presents the first demonstration of SWE change retrieval using spaceborne repeat-pass L-band InSAR observations from the Chinese Lutan-1 mission. The study area focused on the Altay region in Xinjiang, China, during the winter of 2023–2024. Continuous interferometric pairs with 4/8-day temporal baselines are processed for phase changes and then estimate SWE variations. The retrieved SWE change shows a good agreement with in-situ SWE observations during the dry snow period (January 12 to February 9, 2024), with a Root Mean Square Error (RMSE) of 9 mm and a correlation coefficient (R) of 0.48 for the 4-day temporal baselines. However, a heavy snowfall event observed from February 9 to 17, 2024, induced severe decorrelation, leading to phase unwrapping errors that pose a challenge to SWE retrieval. To address the decorrelation mechanism of snow, the InSAR coherence model for snow is established based on the assumption of a bivariate Gaussian distribution for the ground and snow surface. The time-series modeled coherence shows a consistent trend with the observed Lutan-1 coherence, capturing effectively the decorrelation process caused by snowfall events and snow compaction processes. Furthermore, validation of the modeled coherence against Lutan-1 observations shows a strong agreement (R=0.87) over the entire study period from January 12 to March 28, 2024.

Overall, this study demonstrates the capability of spaceborne L-band InSAR with short revisit intervals to effectively retrieve SWE change under appropriate snow conditions. However, the retrieval accuracy is significantly constrained by severe decorrelation during heavy snowfall events. These results highlight both the potential and challenges of operational SWE monitoring from existing and upcoming L-band SAR missions such as Chinese Lutan-1, NASA’s NISAR, JAXA’s ALOS-4, and ESA’s ROSE-L, which are characterized by short repeat cycles, wide swath coverage, and high spatial resolution.

How to cite: Zhou, J., Lei, Y., Pan, J., Li, W., and Shi, J.: Snow Water Equivalent retrieval and InSAR Coherence modeling using L-band Lutan-1 data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20729, https://doi.org/10.5194/egusphere-egu26-20729, 2026.

EGU26-21369 | ECS | PICO | HS6.1

Enhancing Snow Dynamics Monitoring in the Moroccan High Atlas Using Combined Optical and Microwave Satellite Observations 

Hamza Ouatiki, Chaimae Miorqi, Amal Lhimer, and Abdelghani Chehbouni

The seasonal dynamics of snow in Morocco's High Atlas Mountains play a crucial role in the region's water supply, particularly through snowmelt runoff and groundwater recharge in a semi-arid context. Snowmelt provides a significant amount of water to surface and groundwater reservoirs, especially during the summer when precipitation is very rare. However, monitoring snow cover and melt processes in this region remains difficult due to complex topography, high spatial variability, frequent cloud cover in winter, and limited in situ observations. To this end, in this study, we examine the synergistic use of optical and microwave satellite data to improve the monitoring of snow dynamics in the High Atlas.

Optical observations from the Moderate Resolution Imaging Spectroradiometer (MODIS) provide high temporal resolution estimates of snow cover extent, but they are limited by cloud contamination and variable illumination conditions in mountainous terrain. To overcome these limitations, microwave observations from the Sentinel-1 and the Global Microwave Imager (GMI)/Tropical Microwave Imager (TMI) are integrated. The combined optical-microwave framework enables us to improve the temporal continuity and robustness of dynamic snow retrievals, allowing for better characterization of snow accumulation and melt phases across elevation gradients in the High Atlas Mountains, under both clear and cloudy conditions.

The results show that the multi-sensor approach significantly improved the temporal continuity and reliability of snow dynamics monitoring compared to single-sensor approaches. The integration of microwave data allowed for consistent identification of accumulation and melt events, particularly during cloudy periods when MODIS data are not available. In particular, it allowed for better detection of rapid snow events that are often missed by optical data alone and also reduced uncertainty in estimates of snow cover duration, which is essential for assessments of water availability in the High Atlas Mountains. Overall, the approach developed here offers significant potential for improving hydrological modeling and quantifying the contribution of snowmelt to water reservoir storage in semi-arid mountainous regions where data are scarce.

How to cite: Ouatiki, H., Miorqi, C., Lhimer, A., and Chehbouni, A.: Enhancing Snow Dynamics Monitoring in the Moroccan High Atlas Using Combined Optical and Microwave Satellite Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21369, https://doi.org/10.5194/egusphere-egu26-21369, 2026.

EGU26-807 | ECS | Posters on site | GM2.5

Deep-learning classification of cave-floor surface types from LiDAR data for detailed cave mapping 

Michaela Nováková, Jozef Šupinský, and Jozef Širotník

High-resolution 3D mapping of subterranean environments remains challenging due to their complex geometry, low-light conditions, and restricted accessibility. Among these environments, caves represent particularly demanding settings where detailed spatial documentation is essential for monitoring processes, supporting exploration and conservation efforts. Laser scanning has become a key technique for capturing accurate and detailed 3D representations of caves that form the basis for this heritage documentation and multidisciplinary research. Despite these advances, the creation of cave maps still commonly relies on traverse-line measurements and field sketches, later digitized using specialized cave-surveying software. In recent years, LiDAR data have been used for deriving the cave extent. While this method effectively captures the general geometry of cave passages, the delineation of cave-floor units, sediments, speleothems, rock blocks, and other features remains largely manual and relies heavily on the surveyor’s interpretation. As a result, feature boundaries vary between authors, and detailed cave-surface representation lacks reproducibility that is problematic for long-term documentation. In this study, we explore the use of deep-learning semantic segmentation for classifying selected cave-floor surface types based on geometric features derived from LiDAR data. Building on previous work focused on semi-automatic cave-map generation from LiDAR point clouds, we extend the workflow from deriving cave extent and floor morphology toward the automated interpretation of surface materials and forms. The method was tested on several common cave-floor surface types, including clastic sediments, flowstone, and bedrock, as well as artificial surfaces and objects typical in showcaves. The resulting classifications show that deep-learning models can distinguish surfaces with subtle geometric differences and produce consistent, reproducible delineations of units that are traditionally mapped by hand. Compared with manual digitization, the approach reduces subjectivity and provides a scalable way to generate polygonal layers used in speleocartographic workflows.

How to cite: Nováková, M., Šupinský, J., and Širotník, J.: Deep-learning classification of cave-floor surface types from LiDAR data for detailed cave mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-807, https://doi.org/10.5194/egusphere-egu26-807, 2026.

EGU26-1968 | ECS | Posters on site | GM2.5

Comparative Analysis of 30-m DEM Products for Hydrological Applications: A Case Study in the Flinders Catchment Australia 

Laleh Jafari, Ben Jarihani, Jack Koci, Ioan Sanislav, and Stephanie Duce

Digital Elevation Models (DEMs) are fundamental to hydrological modelling, watershed delineation, flood hazard assessment, and resource management. However, the reliability of these applications depends heavily on the vertical accuracy of the DEMs. Although several global DEM products with 30-m spatial resolution are widely available, variations in sensor technology, data acquisition methods, and surface characteristics can significantly influence their accuracy and suitability for hydrological studies. This research provides a comparative evaluation of five commonly used global DEMs—TanDEM-X, ASTER GDEM, SRTM, Copernicus DEM, and ALOS World 3D—by assessing their vertical accuracy against high-resolution airborne LiDAR data and ICESat-2 ATL06 measurements. The findings aim to inform best practices for selecting DEMs in hydrological modelling and catchment-scale applications, particularly in data-scarce regions.

The Flinders River catchment in northern Queensland was selected as the critical test area for evaluating how DEM errors propagate into hydrological calculations. This region is characterised by low rainfall and pronounced topographic variability, encompassing flat lowland plains, dissected upland terrain, and localised areas of steep slopes. All DEMs were standardised to a common horizontal and vertical reference framework and co-registered with the test datasets to eliminate systematic discrepancies. ICESat-2 ATL06 data were rigorously filtered to retain only the highest-quality measurements, based on a combination of quality flags, topographic slope thresholds, and signal strength criteria in vegetated areas.

Elevation differences were computed at matched locations, and DEM performance was evaluated using key statistical metrics, including bias, root mean square error (RMSE), mean absolute error (MAE), median error, and standard deviation. To provide a more comprehensive assessment, error behaviour was analysed in relation to terrain slope and catchment characteristics, highlighting zones most vulnerable to error propagation in flow routing and watershed delineation. Systematic patterns in DEM error were further examined with respect to sensor characteristics under varying landscape conditions.

Results indicate that TanDEM-X and Copernicus DEM exhibit the highest vertical accuracy, closely aligning with ICESat-2 and LiDAR observations, whereas ASTER GDEM and SRTM show larger mean errors, particularly in dissected or mountainous terrain. These findings suggest that TanDEM-X and Copernicus DEM are preferable for hydrology-focused applications in semi-arid basins, while ASTER and SRTM should be used cautiously where precise modelling is required. The study underscores the importance of DEM accuracy evaluation in relation to basin characteristics, as errors can significantly influence hydrological modelling outcomes.

How to cite: Jafari, L., Jarihani, B., Koci, J., Sanislav, I., and Duce, S.: Comparative Analysis of 30-m DEM Products for Hydrological Applications: A Case Study in the Flinders Catchment Australia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1968, https://doi.org/10.5194/egusphere-egu26-1968, 2026.

EGU26-3936 | Posters on site | GM2.5

Historical Images for Surface Topography Reconstruction Intercomparison eXperiment (Historix) 

Amaury Dehecq, Friedrich Knuth, Joaquin Belart, Livia Piermattei, Camillo Ressl, Robert McNabb, and Luc Godin

Historical film-based images, acquired during aerial campaigns since the 1930s and from satellite platforms since the 1960s, provide a unique opportunity to document changes in the Earth’s surface over the 20th century. Yet, these data present significant and specific challenges, including complex distortions in the scanned image and poorly known exterior and/or interior camera orientation. In recent years, semi- or fully-automated approaches based on photogrammetric and computer vision methods have emerged (e.g., Knuth et al., 2023; Dehecq et al., 2020; Ghuffar et al., 2022), but their performance and limitations have not yet been evaluated in a consistent way.

The ongoing “Historical Images for Surface Topography Reconstruction Intercomparison eXperiment (Historix)” project aims at comparing existing methods for processing stereoscopic historical images and harmonizing processing tools.

Within this experiment, participants are provided with a set of historical images and available metadata and invited to return a point cloud and estimated camera parameters. We selected two study sites near Casa Grande, Arizona, and south Iceland, chosen for their  good availability of historical images and variety of terrain types. For each site, we selected 3 sets of film-based images acquired in the 1970s or 80s, overlapping in space and time: aerial images with fiducial marks from publicly available archives and 2 image sets from the American Hexagon (KH-9) reconnaissance satellite missions acquired by the mapping camera (KH-9 MC) and panoramic camera (KH-9 PC). The submitted elevation data will be cross-validated across different image sets and participant submissions, as well as against reference elevation data over stable terrain. The spread in the retrieved elevations will be analysed with respect to image type, terrain type and processing methods to highlight the strengths and limitations of the different approaches.

In this presentation, we will introduce the experiment design, the selected benchmark dataset, the current methodologies and the preliminary results of the intercomparison. Finally, we will present some of the open-source code that exist or are being developed to process historical images.

How to cite: Dehecq, A., Knuth, F., Belart, J., Piermattei, L., Ressl, C., McNabb, R., and Godin, L.: Historical Images for Surface Topography Reconstruction Intercomparison eXperiment (Historix), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3936, https://doi.org/10.5194/egusphere-egu26-3936, 2026.

EGU26-4849 | ECS | Orals | GM2.5

Historical aerial imagery–derived Digital Elevation Models and orthomosaics for glacier change assessment in the western Antarctic Peninsula since 1989 

Vijaya Kumar Thota, Thorsten Seehaus, Friedrich Knuth, Amaury Dehecq, Christian Salewski, David Farías-Barahona, and Matthias H.Braun

The Antarctic Peninsula (AP) is a hotspot of global warming, with pronounced atmospheric warming reported during the 20th century. Although it is critical in terms of climate change studies, the mass balance of glaciers prior to 2000 remains poorly constrained. Existing mass balance estimates are further characterized by high uncertainties due to a lack of observations. In contrast, more than 30000 historical images in archives are the sole direct observations to quantify past glacial changes and their contribution to sea-level rise. 

In this study, we present a unique, timestamped, high-resolution Digital Elevation Model (DEM) and orthomosaic dataset, derived from aerial imagery that covers about 12000 km2 area on the western Antarctic Peninsula and surrounding islands between 66–68° S. We used a film-based aerial image archive from 1989 acquired by the Institut für Angewandte Geodäsie (IfAG), and is kept in the Archive for German Polar Research at the Alfred Wegener Institute, Germany, to generate the historical DEMs and orthoimages. The historical DEMs were co-registered to the Reference Elevation Model of Antarctica (REMA) mosaic on stable terrain. Our historical DEMs have vertical accuracies better than 6 m and 8 m with respect to modern elevation data, REMA, and ICESat-2, respectively. We have made this dataset publicly available at  https://doi.org/10.5281/zenodo.16836526.

Initial mass balance estimates from DEM differencing of our 1989 DEM with recent surfaces from REMA strip DEMs show a near-constant ice mass despite widespread glacier frontal retreat and thinning. We hypothesize that low-elevation ice thickness loss in this period is largely compensated by higher surface mass balance in higher areas. However, this regime appears to be changing, with glaciers transitioning toward increased dynamic activity with enhanced mass loss, and higher ice fluxes.

How to cite: Thota, V. K., Seehaus, T., Knuth, F., Dehecq, A., Salewski, C., Farías-Barahona, D., and H.Braun, M.: Historical aerial imagery–derived Digital Elevation Models and orthomosaics for glacier change assessment in the western Antarctic Peninsula since 1989, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4849, https://doi.org/10.5194/egusphere-egu26-4849, 2026.

Quantifying pebble size, shape, and roundness is fundamental to
understanding sediment transport and abrasion in fluvial systems, yet
remains challenging in natural, densely packed settings.  Most existing
approaches rely on 2D imagery and therefore fail to capture true
three-dimensional morphology. Here, we present a curvature-based instance
segmentation framework for reconstructed surface meshes and demonstrate its
role as a key step enabling 3D roundness and orientation analysis.

In our approach, individual pebbles are detected directly from 3D surface
reconstructions using curvature features, without prior shape assumptions.
Validation against high-resolution reference models yields a high detection
precision of 0.98, with remaining errors mainly due to under-segmentation
in overly smooth reconstructions.  Estimates of 3D pebble orientation are
strongly controlled by the represented surface area, highlighting both the
potential and current limitations of orientation retrieval from incomplete
surface segments.

We illustrate how reliable segmentation allow downstream 3D shape and
roundness analyses that are not accessible in 2D, including curvature-based
surface metrics and volumetric descriptors. Example fluvial scenes
demonstrate that segmentation quality directly controls the stability of
roundness estimates and their geomorphic interpretation. Our results
establish curvature-based 3D pebble segmentation as a methodological
foundation for reproducible analyses of pebble shape, roundness, and
orientation in natural river systems.

How to cite: Rheinwalt, A. and Bookhagen, B.: Curvature-based pebble segmentation as a foundation for 3D roundness and orientation analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5922, https://doi.org/10.5194/egusphere-egu26-5922, 2026.

Currently available global Digital Elevation Model (DEM) surfaces are either derived from the stereoscopic exploitation of multispectral satellite imagery, point-wise laser altimetry measurements or the interferometric processing of bistatic synthetic aperture radar data, but only radar data allows the acquisition of a global product in a reasonable timeframe. The public private partnership of DLR and Airbus in the TanDEM-X mission paved the ground for the WorldDEM product line and its derivatives such as the Copernicus DEM. Both datasets are based on data acquisitions from December 2010 to January 2015, manual and semi-automated DEM editing procedures and represent a very accurate, very consistent and only pole-to-pole DEM data set. The Copernicus DEM is available with a free-and-open licence.

Various ecosystems such as the geosphere, biosphere, cryosphere and anthroposphere are subject to continuous changes which demand the monitoring of Earth’s topography in regular updates of global Digital Elevation Model data. The WorldDEM Neo product represents the successor of the aforementioned WorldDEM but is based on a fully-automated editing & production process and newer data: the on-going TanDEM-X mission is expected to operate until 2028 and has created an archive of up-to-date DEM scenes ready for integration into a new global DEM coverage (>90% of global landmass acquired between 2017 and 2021; ~60% of global landmass acquired again between 2021 and 2025). In conjunction with continuous improvements of the fully-automated production processes, a new global DEM coverage of WorldDEM Neo is produced early 2026. DEM applications such as the orthorectification of raw satellite imagery will benefit from the availability of an accurate and up-to-date global DEM dataset. Other applications such as multi-temporal 3D change analysis based on a single satellite mission (TanDEM-X) are possible and support the understanding of environmental changes thanks to the 3rd dimension. The rapid availability of the error-compensated WorldDEM Neo Digital Surface Model (DSM) and bare-ground Digital Terrain Model (DTM) after raw data acquisition serve various applications of global DEMs. Future acquisitions of the on-going TanDEM-X mission (until 2028) allow the processing of final and up-to-date DSM and DTM coverages at the end of the mission lifetime.

The presentation comprises a short look into the history with its manual & semi-automated DEM editing procedures. The main focus will be on the fully-automated production processes for truly global DSM & DTM coverages. Accuracy metrics, 3D change statistics between the different global coverages but also visual impressions of the various global DEM coverages will be addressed, too. On-going challenges with interferometry-based elevation data are part of an outlook and different error compensation strategies (e.g. height reconstruction from radar amplitude data based on machine-learning techniques) are highlighted.

How to cite: Fahrland, E. and Schrader, H.: Updating and upgrading a global Digital Elevation Model - the fully automated production of WorldDEM Neo with acquisitions until 2025, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6660, https://doi.org/10.5194/egusphere-egu26-6660, 2026.

EGU26-9007 | ECS | Orals | GM2.5

Use of time-lapse photogrammetry to capture substantial accumulation rates on an on-glacier avalanche deposit  

Marin Kneib, Patrick Wagnon, Laurent Arnaud, Louise Balmas, Olivier Laarman, Bruno Jourdain, Amaury Dehecq, Emmanuel Le Meur, Fanny Brun, Andrea Kneib-Walter, Ilaria Santin, Laurane Charrier, Thierry Faug, Giulia Mazzotti, Antoine Rabatel, Delphine Six, and Daniel Farinotti

Avalanches are critical contributors to the mass balance and spatial accumulation patterns of mountain glaciers. While gravitational snow redistribution models predict high localized accumulation, these predictions lack field validation due to the difficulty of monitoring highly dynamic avalanche cones. Here, we present two years of high-resolution monitoring of a large avalanche cone in the accumulation area of Argentière Glacier (French Alps). To capture these dynamics, we employed a multi-sensor approach: Uncrewed Aerial Vehicle (UAV) surveys and a time-lapse photogrammetry array consisting of 7 low-cost cameras deployed ~1 km away from the cone. The distance of the sensors from the surveyed area, its geometry (>30°), its surface characteristics (smooth snow surface) and the absence of fixed stable terrain due to the surrounding headwalls being episodically covered in snow made this environment particularly challenging for the photogrammetry methods applied. Point clouds and Digital Elevations Models were produced at a two-week resolution using Structure-from-Motion photogrammetry in Agisoft Metashape v1.8.3. with the alignment being constrained with Pseudo Ground Control Points. We could further co-register all point clouds to a September UAV acquisition with the Iterative Closest Point algorithm from the open-source project Py4dgeo, using automatically-derived stable ground from the RGB information of the images.

Methodological validation shows that while side-looking time-lapse photogrammetry captures the overall trend, it tends to underestimate elevation changes compared to UAV data, with biases up to 1.8 m and standard deviations of 2–6 m. Winter-time acquisitions with low light conditions over smooth snow surfaces also lead to reduced correlation over the cone. Despite these uncertainties, our results reveal extreme spatial variability in accumulation. The top of the cone is the most active zone, exhibiting elevation changes of ~30 m annually and a strong accumulation of 60 m w.e. between March 2023 and 2025 when accounting for the ice flow—roughly 15 times the annual mass balance recorded by the GLACIOCLIM program in the nearby accumulation area not affected by avalanche deposits. We identify a topographical threshold for snow storage: the upper cone fills early in the season until reaching a critical slope of ~35°, after which subsequent avalanches bypass the apex to deposit mass at the cone’s base. From May onwards, mass redistribution is further modulated by the development of surface channels. Our findings demonstrate that time-lapse photogrammetry is a viable tool for monitoring dynamic glacier surfaces and provide rare empirical evidence of the dominant role avalanches play in glacier mass budgets.

How to cite: Kneib, M., Wagnon, P., Arnaud, L., Balmas, L., Laarman, O., Jourdain, B., Dehecq, A., Le Meur, E., Brun, F., Kneib-Walter, A., Santin, I., Charrier, L., Faug, T., Mazzotti, G., Rabatel, A., Six, D., and Farinotti, D.: Use of time-lapse photogrammetry to capture substantial accumulation rates on an on-glacier avalanche deposit , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9007, https://doi.org/10.5194/egusphere-egu26-9007, 2026.

EGU26-9167 | ECS | Posters on site | GM2.5

Optimizing SfM workflows for continuous river bank monitoring: evaluating image alignment accuracies across diverse environmental conditions 

László Bertalan, Lilla Kovács, Laura Camila Duran Vergara, Dávid Abriha, Robert Krüger, Xabier Blanch Gorriz, and Anette Eltner

River bank erosion represents a dynamic geomorphic hazard, particularly in meandering channels where migration rates threaten critical infrastructure and agricultural land. While our previous work on the Sajó River (Hungary) established a novel, low-cost monitoring framework utilizing Raspberry Pi (RPi) cameras for near-continuous observation, the reliability of photogrammetric reconstruction under uncontrolled outdoor conditions remains a critical challenge. This study presents a systematic evaluation of the accuracy constraints inherent in automated Structure-from-Motion (SfM) processing pipelines, with a specific focus on optimizing image alignment across a wide range of scene conditions.

To determine the robustness of RPi imagery, we conducted a comprehensive sensitivity analysis of the SfM-based image alignment phase. We systematically tested over 120 variations of processing parameters, manipulating keypoint and tie-point limits, upscaling factors, and masking strategies. The implementation of rigorous masking was critical, as the imagery is geometrically challenging: the moving river surface in the foreground and the sky in the background occupy the majority of the field of view, leaving only a narrow, static fraction of the image relevant for reliable 3D reconstruction. These combinations were evaluated against a dataset representing the full range of environmental variability, including clear, cloudy, dark, foggy, overexposed, and rainy conditions, as well as distinct hydrological states such as low flows, flood events, and snow cover.

Preliminary results indicate that a specific balance of 30,000 keypoints and 5,000 tie points (ratio 6.0) optimizes reconstruction fidelity, achieving an RMS error of 0.75 pixels under clear weather conditions. Notably, the system demonstrated unexpected robustness in low-light scenarios, maintaining consistent error margins of 1.17–1.18 pixels across various configurations. Conversely, scaling up these limits beyond the optimum yielded diminishing returns, confirming that higher computational loads do not necessarily equate to improved geometric accuracy. Furthermore, we applied gradual selection algorithms to filter sparse point clouds, removing unreliable points based on reconstruction uncertainty to isolate the most geometrically valid features.

The crucial final phase of this research bridges the gap between digital reconstruction and physical reality. We validate the optimized SfM-based point clouds by comparing them directly against high-precision Terrestrial Laser Scanning (TLS) data acquired during two previous campaigns and upcoming field surveys. This multi-temporal comparison allows us to quantify specific error margins for volumetric and horizontal material displacement calculations. By defining these accuracy constraints, we establish a validated protocol for calculating erosion volumes during high-flow events, ensuring that automated, low-cost monitoring systems can provide actionable, high-precision data for river management even under adverse environmental conditions.

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The research was funded by the DAAD-2024-2025-000006 project-based research exchange program (DAAD, Tempus Public Foundation).

How to cite: Bertalan, L., Kovács, L., Duran Vergara, L. C., Abriha, D., Krüger, R., Blanch Gorriz, X., and Eltner, A.: Optimizing SfM workflows for continuous river bank monitoring: evaluating image alignment accuracies across diverse environmental conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9167, https://doi.org/10.5194/egusphere-egu26-9167, 2026.

Long-term observations of glacier mass change provide a key indicator of atmospheric warming and are essential for understanding glacier behaviour and responses to climate forcing. Archived aerial photographs represent an underutilised source of historical information from which three-dimensional surface geometry can be reconstructed to quantify past glacier change. This approach is particularly valuable in Antarctica, where surface-elevation change prior to the 1990s remains poorly constrained due to limited pre-satellite altimetry and a scarcity of reliable Ground Control Points (GCPs). As a result, historic mass-balance estimates have largely relied on climate reanalysis and modelling.

Advances in photogrammetric techniques have substantially improved the efficiency and accuracy of Digital Elevation Models (DEMs) derived from historical aerial imagery. Here, we present a newly compiled inventory of Antarctic aerial surveys conducted throughout the twentieth century, documenting their spatial and temporal coverage to identify regions suitable for DEM reconstruction. Then, building on established workflows, we show newly constructed DEMs for three glaciers that formerly fed the Larsen A Ice Shelf on the Antarctic Peninsula, capturing surface geometry both before and after its collapse in 1995. These reconstructions reveal heterogenous glacier responses to reduced buttressing, controlled by local morphology and consistent with previous regional observations.

How to cite: Rowe, E., Willis, I., and Fenney, N.: Compiling an Inventory of Historic Antarctic Aerial Photographs to Measure Long-Term Glacial Mass Balance Change from Digital Elevation Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13015, https://doi.org/10.5194/egusphere-egu26-13015, 2026.

EGU26-13875 | Posters on site | GM2.5

Using high-resolution bathymetric data from a multibeam sonar acquisition to map and analyse geomorphical underwater structures in the proglacial Grastallake in the Horlachtal valley/ Ötztal Alps 

Florian Haas, Manuel Stark, Jakob Rom, Lucas Dammert, Till Kohlhage, Toni Himmelstoss, Diana-Eileen Kara-Timmermann, Moritz Altmann, Carolin Surrer, Korbinian Baumgartner, Peter Fischer, Sarah Betz-Nutz, Tobias Heckmann, Norbert Pfeifer, Gottfried Mandlburger, and Michael Becht

As part of the DFG research group “Sensitivity of high alpine geosystems to climate change since 1850” (SEHAG), high-resolution multibeam sonar data was collected from the proglacial Grastallake in the Ötztal valley during a boat survey in the summer of 2025. The Grastallake has an area of approximately 63,000 m², a maximum depth of approximately 16 m, and lies at an altitude of 2,584 m. The lake is situated in a former cirque, and its shores and the surrounding are partly composed of loose material and partly of solid rock. In the western part, there is a large whaleback with already known Egesen-moraines on top. On the southern and eastern shores, larger active debris flow cones are coupled to the lake, with meltwater runoff from the higher Grastalferner glacier flowing into the lake as a perennial stream via the eastern debris flow cone. Due to the permanent inflow from the glacier and the topographic conditions of the catchment area, the eastern debris flow cone is very active and has intensively been reshaped by several extreme debris flow events during the last years.

The bathymetric data was collected using a Norbit multibeam sonar (WBMS), which was supplemented by an SBG INS system (dual GNSS patch antenna system, SBG Eclipse D) by Kalmar Systems. Since the underwater topography of the lake was unknown and its high turbidity due to the glacier inflow, the first step was to conduct a rough survey of the lake. This step made it possible to create a coarse depth map on site in order to identify spots with shallow water, determine the system settings, and draw up a navigation plan along strips. After field work the recorded data was processed using Quinertia for trajectory calculation and Opals for strip adjustment. This resulted in a final 3D point cloud with an average point density of 400 points per square meter, which was converted to raster data in order to perform spatial analyses.

Using the data, geomorphological forms were mapped in a first step. In addition to a previously unknown late glacial moraine section, the underwater deposits of recent debris flows became visible. In addition to mapping, geomorphological structures were used for spatial analysis, such as comparing the depositions of debris flows above and below the water. Since the data is very well suited for mapping underwater structures, this case study demonstrates the enormous potential of bathymetric data acquired by multibeam sonar measurements, that has rarely been used for geomorphological studies to date. Multitemporal analysis in the sense of a 4D analysis could only be carried out to a limited extent in this case study. However, with the data now available, multitemporal analysis, i.e., quantification of sediment input into lakes, will also be possible in the future. This would then enable assessments to be made of the hazard potential of newly formed lakes in the proglacial area and of their lifespan. 

How to cite: Haas, F., Stark, M., Rom, J., Dammert, L., Kohlhage, T., Himmelstoss, T., Kara-Timmermann, D.-E., Altmann, M., Surrer, C., Baumgartner, K., Fischer, P., Betz-Nutz, S., Heckmann, T., Pfeifer, N., Mandlburger, G., and Becht, M.: Using high-resolution bathymetric data from a multibeam sonar acquisition to map and analyse geomorphical underwater structures in the proglacial Grastallake in the Horlachtal valley/ Ötztal Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13875, https://doi.org/10.5194/egusphere-egu26-13875, 2026.

EGU26-17031 | ECS | Posters on site | GM2.5

High-precision point cloud generation for forest inventory: Integrating GNSS-RTK and SLAM for handheld laser scanning 

Carolin Rünger, Stefan Binapfl, Ferdinand Maiwald, Robert Krüger, and Anette Eltner

In recent years, forest management and inventory have increasingly relied on handheld personal laser scanners (H-PLS) for capturing flexible three-dimensional data. These systems have become essential for extracting critical tree attributes, such as diameter at breast height (DBH) and tree height. Most traditional H-PLS systems utilize Simultaneous Localization and Mapping (SLAM), which fuses LiDAR and Inertial Measurement Unit (IMU) data to reconstruct environments. However, SLAM is based on relative sensor measurements, which inherently causes accumulated errors and trajectory drift. In complex forest environments, similar-looking stems and moving vegetation can further confuse the mapping process, resulting in distorted point clouds or duplicated stems that reduce the accuracy of extracted tree attributes.

While Global Navigation Satellite System (GNSS)-based Real-Time Kinematic (RTK) positioning provides centimetre-level absolute accuracy and usually drift-free trajectories, its application in forestry is critically hindered by signal obstruction in dense canopies. The integration of GNSS-RTK and SLAM offers a robust and synergetic solution to these challenges, allowing one method to compensate for the failures of the other. A promising development in this field is an H-PLS system that integrates GNSS-RTK, IMU, LiDAR, and camera measurements to generate georeferenced point clouds directly in the field. This hybrid approach utilizes LiDAR and camera data to maintain positioning during GNSS outages and utilizes RTK information to re-initialize and correct the trajectory once the signal is restored.

Our study evaluates whether this integrated GNSS-RTK SLAM approach improves point cloud geometry and tree attribute extraction compared to traditional SLAM methods without GNSS integration. We conducted a field campaign in a mixed forest stand during the leaf-off period to simulate realistic operating conditions with alternating GNSS visibility. The performances of a SLAM-only and a SLAM + GNSS-RTK H-PLS were validated against highly accurate terrestrial laser scanning (TLS) reference data. The analysis involved tree segmentation to assess individual tree identification and the derivation of DBH, stem positions, and tree heights. Furthermore, we investigated internal geometric quality by analysing local noise levels using cross-sectional residuals relative to fitted circles and assessed spatial homogeneity to identify artifacts like duplicated stems or gaps.

Initial results indicate that the SLAM + GNSS-RTK H-PLS system provides DBH estimates comparable to TLS, with observed differences of 6.3 mm and 1.17 cm for major and minor axes, respectively. Despite slight overestimations due to scattering, the significantly reduced acquisition time makes this integrated system an efficient alternative for forestry applications. These findings contribute to a better understanding of how integrated positioning systems can enhance mobile laser scanning workflows and support the development of autonomous, high-precision forest mapping solutions.

How to cite: Rünger, C., Binapfl, S., Maiwald, F., Krüger, R., and Eltner, A.: High-precision point cloud generation for forest inventory: Integrating GNSS-RTK and SLAM for handheld laser scanning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17031, https://doi.org/10.5194/egusphere-egu26-17031, 2026.

EGU26-17484 | Orals | GM2.5

Permanent terrestrial laser scanning for environmental monitoring 

Roderik Lindenbergh, Sander Vos, and Daan Hulskemper

Many topographic scenes demonstrate complex dynamic behavior that is difficult to map and understand. A terrestrial laser scanner fixed on a permanent position can be used to monitor such scenes in an automated way with centimeter to decimeter quality at ranges of up to several kilometers. Laser scanners are active sensors, and can continue operation during night. Their independence from surface texture properties ensures in principle that they provide stable range measurements for varying surface conditions.

Recent years have seen an increase in the employment of such systems for different applications in environmental geosciences, including forestry, glaciology and geomorphology. This employment resulted in a new type of 4D topographic data sets (3D point clouds + time) with a significant temporal dimension, as such systems can acquire thousands of consecutive epochs.

However, extracting information from these 4D data sets turns out to be challenging, first, because of insufficient knowledge on error budget and correlations, and second, because of lack of algorithms, benchmarks, and best-practice workflows.

The presentation will showcase recently active systems that monitored a forest, a glacier, an active rockfall site and a sandy beach respectively. Data from these systems will be used to illustrate different systematic challenges that include instabilities of the sensor system, meteorological and atmospheric influence on the data product and the maybe surprising need for alignment of point clouds from different epochs.

In addition, different ways to extract information from these 4D data sets will be discussed, in connection with particular applications. While bi-temporal change detection is often a starting point for exploring 4D data, several methods are being developed that truly exploit the extensive time dimension, including tracking, trend analysis, time series clustering and spatio-temporal region growing.

Lessons learned from experiences with these systems in different domains lead to several recommendations for future employment considering field of view design, auxiliary sensors (e.g. IMU, camera, weather station) and the possible deployment of low-cost alternatives, thereby providing a view on the near future of permanent laser scanning.

Reference

Lindenbergh, R., Anders, K., Campos, M., Czerwonka-Schröder, D., Höfle, B., Kuschnerus, M., Puttonen, E., Prinz, R., Rutzinger, M., Voordendag, A & Vos, S. (2025). Permanent terrestrial laser scanning for near-continuous environmental observations: Systems, methods, challenges and applications. ISPRS Open Journal of Photogrammetry and Remote Sensing, 17, 100094. DOI: 10.1016/j.ophoto.2025.100094

How to cite: Lindenbergh, R., Vos, S., and Hulskemper, D.: Permanent terrestrial laser scanning for environmental monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17484, https://doi.org/10.5194/egusphere-egu26-17484, 2026.

Beachrocks are cemented coastal deposits formed within the intertidal zone by the precipitation of magnesium-rich calcium carbonate. They constitute important paleogeographic and paleoclimatic markers, as they allow the reconstruction of past shoreline evolution. In addition, beachrocks influence current coastal dynamics and represent valuable geological heritage and ecological reservoirs that require preservation.

This study focuses on a sequence of multiple beachrock levels located along the Catalan Coast (NE Iberian Peninsula). The system consists of a complex sequence of submerged beachrocks with a wide formation range, situated at water depths between −0.25 m and −48 m below the current sea level. These deposits exhibit lateral continuity of up to 4.5 km and are characterized by reduced thicknesses and low geomorphic expression. The underlying substrate is composed of unconsolidated marine sediments. In certain sectors, a spatial overlap with Posidonia oceanica meadows occurs.

The aforementioned characteristics hinder their cartographic representation using traditional methods, such as aerial image interpretation and hillshade maps derived from bathymetric data, particularly for thin structures located at greater depths and in areas where Posidonia oceanica meadows are present.

The aim of this study is to evaluate the usefulness of the Red Relief Image Map (RRIM) method as an alternative quantitative terrain visualization tool for the cartography of submerged beachrocks. This method is based on the quantitative attribute openness, which expresses the degree of dominance or enclosure of a location on an irregular surface and enhances concave (negative openness) and convex (positive openness) features. Using this attribute, the RRIM method combines three main elements: topographic slope, positive openness and negative openness, allowing the visualization of subtle, low-relief topographic structures on apparently flat surfaces.

Using this approach, this study aims to improve the identification and cartographic delineation of submerged beachrock levels and to define optimal visualization parameters that contribute to a better understanding of the beachrock sequence.

How to cite: Vicente, M.-A., Mencos, J., and Roqué, C.: Testing the Red Relief Image Maps methodology to enhance the beachrock cartography in Torredembarra coast (Catalan coast, West  Mediterranean Sea), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17571, https://doi.org/10.5194/egusphere-egu26-17571, 2026.

EGU26-17927 | ECS | Posters on site | GM2.5

Long-term glacier elevation change at Gran Campo Nevado since 1945  

Lucas Kugler, Camilo Rada, Clare Webster, Jan Dirk Wegner, Etienne Berthier, and Livia Piermattei

Scanned historical aerial photographs acquired with film cameras from the early twentieth century to the early 2000s are the longest and richest archive of Earth observation data for reconstructing past topography. Those with stereoscopic acquisition enable the generation of Digital Elevation Models (DEMs) and orthoimages when processed with photogrammetric techniques, extending the assessment of environmental change beyond the time scale of modern satellite observations.  

In this study, we present a long-term (1945-2020) dataset of glacier surface elevation for the Gran Campo Nevado ice field in southern Chile. The dataset is based on aerial photographs acquired in 1945 using a Trimetrogon camera and in the 1980s and 1990s using nadir-looking film cameras from the Chile60 and Geotec flight campaigns, complemented by a 2020 Pléiades satellite–derived DEM made available through the Pléiades Glacier Observatory program (Berthier et al., 2023). To process the historical photographs, we developed an open-source pipeline that builds on structure-from-motion (SfM) principles and incorporates learning-based feature-detection and matching algorithms, such as SuperPoint and LightGlue. Absolute image orientation is achieved through automated detection of ground control points derived from the Pléiades DEM and orthoimage. DEMs accuracy was evaluated over stable terrain by comparing them with the Pléiades reference DEM. As well, the reconstructed DEMs are compared with those obtained using an established SfM processing workflow (HSfM; Knuth et al., 2023). The resulting DEMs provide a reconstruction of glacier surface elevation spanning more than seven decades, and glacier elevation changes are quantified from the DEM time series. By using reproducible, open-source methodologies, this presentation demonstrates opportunities for the research community to leverage other historical datasets and extend analyses beyond what is possible with modern satellite observations alone. 

How to cite: Kugler, L., Rada, C., Webster, C., Wegner, J. D., Berthier, E., and Piermattei, L.: Long-term glacier elevation change at Gran Campo Nevado since 1945 , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17927, https://doi.org/10.5194/egusphere-egu26-17927, 2026.

EGU26-18399 | ECS | Orals | GM2.5

From badland to bushland? Analysis of geomorphic process dynamics and vegetation development in a sub-humid calanchi area based on high-resolution UAS data (2014-2024). 

Manuel Stark, Annalisa Sannino, Martin Trappe, Jakob Rom, Jakob Forster, Georgia Kahlenberg, Florian Haas, and Francesca Vergari

Badlands are among the most rapidly developing landscapes and exhibit a significant degree of geomorphological activity. In semi-arid/ sub-humid landscapes, specific precipitation dynamics result in particularly rapid geomorphological development. This applies in particular to land cover and geomorphology. This study employs quantitative, multi-temporal analysis to examine the spatio-temporal changes in a sub-humid calanchi badland in the upper Val d'Orcia (Italy) over a period of ten years (2014-2024). Particular emphasis lies on the dynamics of geomorphological processes and topographical changes, while considering the variables of vegetation and precipitation. The analysis encompasses both extreme events and prolonged rainfall lasting several days, which are the primary factors for surface changes in subhumid badlands. The utilisation of UAS SfM-MVS in conjunction with precise dGNSS measurements facilitates high-resolution change detection and landform analysis across five distinct observation periods, each spanning two years (= five DoD). The interactions between vegetation and geomorphological processes are investigated using a semi-automatic mapping approach based on the Triangular Greenness Index (TGI) and the interpretation of topographical changes (DoD). The vegetation analysis are based on high-resolution orthomosaics with a resolution of 0.05 m, while the geomorphic change detection analysis is carried out on 2.5D rasterised digital surface models with a resolution of 0.25 m. The major results are as follows: The mean slope gradient of the entire study site remained largely stable despite certain areas showing enhanced geomorphic activity. The DoD analysis revealed four 'geomorphic hot spots', areas of enhanced geomorphic activity and sediment contribution from the tributaries to the main valley (the major deposition area). The annual erosion rates vary between -0.4 cm (2018-2022) and -4 cm (2022-2024). The observed topographic changes can be attributed primarily to high-magnitude events (complex landslides and debris-like flows) that occur irregularly. The multi-temporal mapping of landforms has revealed a significant reduction in water erosion, with a 50% decrease observed from 35% in 2014 to 17% in 2024. Furthermore, the combination of 2D-mappings and 2.5D DoD-analysis enabled the documentation of a geomorphological process previously unknown in badland areas, namely gravitational bulging. This describes the deformation of sediments in lower-lying clay layers as a response to water infiltration, high swelling capacities of clays and the pressure exerted by the sediment packages lying above them. A significant increase in vegetation cover has been observed, particularly in areas designated as potentially moist and gentle terrain, often the deposition areas from the previous period. In general, vegetation underwent a gradual transition, evolving from a fragmented to a continuous structure, primarily due to the widespread colonisation of the main valley and the landslide pathways.  Although the area affected by erosion processes decreased over the course of the study period, erosion rates remained relatively constant. This indicates a shift from high-frequency to high-magnitude processes in the most recent observation period. Overall, the phase under consideration in this study (2014-2024) can be characterised as a phase of badland stabilisation.

How to cite: Stark, M., Sannino, A., Trappe, M., Rom, J., Forster, J., Kahlenberg, G., Haas, F., and Vergari, F.: From badland to bushland? Analysis of geomorphic process dynamics and vegetation development in a sub-humid calanchi area based on high-resolution UAS data (2014-2024)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18399, https://doi.org/10.5194/egusphere-egu26-18399, 2026.

EGU26-19445 | ECS | Orals | GM2.5 | Highlight

From Static to Dynamic: Modernizing the Sharing of HistoricalPhotogrammetry Datasets 

Felix Dahle, Roderik Lindenbergh, and Bert Wouters

The recovery of historical topography from analogue aerial archives has has become a well-established workflow in geosciences, unlocking high-resolution records of topographic change that were previously inaccessible. However, the standard practice for sharing these results relies on static FTP servers or raw file downloads. Consequently, these datasets often remain difficult to discover, particularly for researchers from other disciplines who cannot easily assess the spatial coverage or relevance of the archive through static file lists. Furthermore, existing web-based visualization solutions often require complex database configurations and advanced full-stack development skills, rendering them inaccessible for many geoscience research groups lacking dedicated software engineers.

In this work, we present a lightweight, open-source web application designed to support the publication of historical photogrammetric data. The design prioritizes portability and ease of deployment for non-developers. Unlike complex Content Management Systems (CMS) that rely on heavy database backends, our tool utilizes a streamlined file-based ingestion pipeline. Researchers can deploy a fully interactive instance by populating a directory structure with standard geospatial vector formats (e.g., Shapefiles, GeoJSON) and point cloud data. The Node.js-based backend automatically parses these inputs to configure the visualization interface, thereby eliminating the need for manual database administration.

We demonstrate the capabilities of the website using a dataset from the Antarctic TMA archive with ~ 250.000 images. The resulting interface facilitates spatio-temporal discovery through an interactive map that visualizes survey footprints, including the residuals between metadata-derived and SfM-estimated positions. This allows users to rapidly assess geometric quality and survey coverage. To extend the platform beyond simple 2D mapping, we present the architectural integration of Potree for browser-based 3D visualization. We discuss the workflow for streaming massive point clouds to the client, a feature designed to transform the website from a passive gallery into an active analytical tool for measurement and validation. Finally, we address the challenge of data distribution by outlining the implementation of a bulk-download utility, structured to allow users to filter and request specific subsets of raw imagery, associated metadata and processed data based on their visual selection.

By providing a self-contained, low-dependency solution, we aim to shift the community standard from static archiving to dynamic, interactive exploration. This tool allows geoscientists to easily share their historical images and reconstructions and make their data truly accessible to the broader scientific community without the overhead of custom software development.

How to cite: Dahle, F., Lindenbergh, R., and Wouters, B.: From Static to Dynamic: Modernizing the Sharing of HistoricalPhotogrammetry Datasets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19445, https://doi.org/10.5194/egusphere-egu26-19445, 2026.

EGU26-20499 | ECS | Posters on site | GM2.5

Detecting desert kites in 3D point clouds by learning anomalies 

Reuma Arav

Desert kites are large prehistoric hunting traps typically composed of two long, low stone walls that converge toward an enclosure.  These structures are widely distributed across the arid and semi-arid margins of the Middle East and Central Asia, exhibiting substantial variability in size, geometry, construction techniques, and topographic setting. To better understand their functionality from the Neolithic to sub-contemporaneous times, terrestrial laser scanning has increasingly been used to capture high-resolution three-dimensional representations of desert kites, enabling detailed characterization of their construction and local terrain setting. However, the kites’ subtle expression, their large spatial extent, and their progressive blending into the natural surface complicate their detection. These difficulties are further exacerbated by variable point density resulting from the alignment of multiple terrestrial scans, unavoidable occlusions caused by topography or vegetation, and the sheer volume of data produced by high-resolution ground-based surveys.  Together, these factors make the reliable identification and analysis of desert kite features within raw terrestrial point clouds a challenge, which requires extensive manual intervention and expert interpretation.

In this study, I present an automated, machine-learning-based approach for highlighting desert kite features directly within 3D point clouds derived from terrestrial laser scanning, without the need for manual annotation or labelled training data. The proposed method is based on the premise that the kites' structures introduce geometric irregularities (anomalies) relative to the surrounding natural surface. Rather than explicitly modelling the kite's form  or imposing predefined shape descriptors, the method learns a representation of the underlying terrain surface directly from the point cloud. This learned representation is then used to reconstruct the surface, which is subsequently compared to the original terrestrial measurements. Local deviations between the reconstructed surface and the original point cloud are quantified, with larger reconstruction errors interpreted as potential surface anomalies indicative of the kite's features. 

The proposed workflow is fully data-driven and unsupervised. It does not rely on prior knowledge of kite geometry, site-specific heuristics, or expert-defined thresholds. Instead, the learning process adapts to the local surface characteristics captured in the input dataset, making it robust to variations in resolution, occlusions, and terrain complexity commonly encountered in terrestrial laser scanning surveys. 

The findings demonstrate that surface-reconstruction-based anomaly detection offers a promising pathway for the automated identification of desert kite features in terrestrial 3D point clouds. More broadly, the approach is applicable to archaeological structures that exhibit weak or subtle geometric signatures. By reducing dependence on manual interpretation and labelled datasets, the method supports more objective, scalable, and reproducible analyses of archaeological landscapes, particularly in complex terrain where anthropogenic features are embedded within natural surfaces.

How to cite: Arav, R.: Detecting desert kites in 3D point clouds by learning anomalies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20499, https://doi.org/10.5194/egusphere-egu26-20499, 2026.

Despite significant advancements in landslide monitoring, landslides occurring on densely forested slopes remain largely unexplored. While conventional subsurface characterization methods (e.g., DPH, CPT, percussion drilling) are often impractical due to limited accessibility and steep rugged terrain, surficial analyses using remote sensing techniques frequently face challenges in capturing high-resolution ground surface data due to occlusion caused by dense vegetation cover as well as technical limitations.
Although trees and forests are generally acknowledged to reduce the probability of landslide occurrence, they are unlikely to prevent or substantially mitigate deep-seated landslides or failures on very steep slopes. Instead, trees may serve as proxies of landslide activity, potentially improving the understanding and monitoring of densely forested slopes. Affected by slope movements, trees experience external growth disturbances and develop characteristic growth anomalies that can be partly attributed to underlying landslide processes.

Multiple studies have demonstrated the feasibility of extracting such external growth disturbances, primarily stem tilting, by assessing the inclination and curvature of tree stems in LiDAR point clouds, greatly building upon previous forestry-related studies exploring the mapping, classification, and derivation of stem parameters such as height and diameter from digital twins. However, the potential to extract externally visible eccentric growth patterns in stem cross-sections at heights of maximum bending, analogous to dendrogeomorphologic tree-ring analyses, as a proxy for landslide activity has not yet been explored. Additionally, the classification of overall tree shape may provide valuable insights into the characteristics of underlying slope movements, but, to the best of the author’s knowledge, this has not been addressed in previous research.

To investigate the potential of automatically extracting tree shape and stem eccentricity from LiDAR data, and to evaluate their suitability as proxies of landslide activity, we introduce an improved two-stage processing pipeline for tree identification and extraction, along with a dedicated framework for digital dendrogeomorphology. Building upon previous work, we compute normal vectors of locally fitted planes and projected point densities to separate trees from the point cloud. To enhance the extraction of complex shaped trees (e.g., S-shaped or pistol-butted) characteristic of landslide-prone slopes, we introduce dynamically adjusted normal vector thresholds derived from estimated stem inclination. After segmenting tree stems from the point cloud, ellipses are fitted at configurable height intervals to determine cross-section centroids. These centroids are then connected as vertices of a 3D polyline, which is subsequently smoothed using a natural spline to represent the generalized stem geometry. Based on the curvature of the resulting polyline, the height of maximum bending is identified, and the corresponding cross-section eccentricity is extracted. In addition, the curvature of the polyline is used to categorically classify overall tree shape.

Our digital dendrogeomorphology approach applied to 3D point clouds enables accurate extraction of stem eccentricity, even for complex tree shapes typical of landslide-prone slopes. When paired with automated tree-shape classification, these data offer insights into slope movement and improve understanding of landslide processes in densely forested environments.

How to cite: Kamaryt, T.-H. and Müller, B.: Tree Geometry as a Potential Proxy for Landslide Activity in Densely Forested Slopes: A LiDAR-Based Digital Dendrogeomorphology Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21238, https://doi.org/10.5194/egusphere-egu26-21238, 2026.

Large-scale infrastructure development in mountain regions produces significant changes in slope morphology and surface processes. However, stability assessments conducted after construction often rely on static or short-duration evaluations. These approaches tend to assume an immediate geomorphic adjustment to human disturbance, which can overlook delayed and nonlinear responses of hillslopes. This study examines terrain adjustments that occur with a time delay following major construction activities in complex mountainous settings. The analysis is based on a series of high-resolution topographic datasets obtained through repeated LiDAR surveys along the Sibiu - Pitești motorway corridor in the Southern Carpathians of Romania. Changes in terrain configuration caused by excavation, filling, drainage alteration, and the unloading of slopes are identified by comparing elevation models and terrain metrics. Instead of focusing solely on deformation located at the site of intervention, the study investigates terrain responses that appear later and in areas situated upslope or laterally from the engineered zones. Findings show that slope instability and surface reorganization often emerge after a measurable time delay, typically reactivating existing geomorphic features such as drainage pathways, slope breaks, and erosional forms. These responses are not random but show a strong dependence on prior landscape conditions and the type of construction-related disturbance. The results emphasize the limitations of early assessments performed shortly after construction, which may fail to capture landscape dynamics relevant for landslide initiation. The study demonstrates the usefulness of repeated LiDAR mapping for detecting evolving terrain responses in engineered mountain landscapes and supports the integration of time-sensitive processes into hazard assessment strategies.

How to cite: Al-Taha, W., Andra-Topârceanu, A., and Mustățea, S.: Delayed slope response to infrastructure-induced landscape modifications in mountainous terrain revealed by high-resolution LiDAR analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21758, https://doi.org/10.5194/egusphere-egu26-21758, 2026.

EGU26-22072 | ECS | Posters on site | GM2.5

Automated photogrammetric reconstruction of Birch Glacier, Switzerland (1946–2025): A high-density time series of topographic change preceding catastrophic glacier collapse 

Friedrich Knuth, Elias Hodel, Holger Heisig, Mauro Marty, Mylène Jacquemart, Andreas Bauder, Jean-Luc Simmen, and Daniel Farinotti

As glaciers retreat, permafrost degrades, and mountains destabilize, modern landscape evolution is increasing the potential for catastrophic events, such as the Birch Glacier collapse on May 28, 2025. To improve our understanding of mass movements in mountainous regions and support future hazard assessment and risk mitigation efforts, we are generating time series of glacier surface elevation change from historical aerial photography provided by the Swiss Federal Office of Topography (Swisstopo). 

In this case study, we leveraged multi-temporal photogrammetric reconstruction and Digital Elevation Model (DEM) coregistration techniques, implemented in the Historical Structure from Motion (HSfM) pipeline, to generate an ~80-year record of self-consistent DEMs and orthoimage mosaics from analog film imagery collected over the Birch Glacier between 1946 and 2010. From 1985 until 2010 we generated nearly annual surface measurements, making this a unique and remarkably dense historical time series. The time series is augmented with modern surface measurements generated from linescan and UAV imagery collected during the period of 2010 to 2025. To quantify the uncertainty of elevation change measurements we compute residuals with respect to the swissSURFACE3D elevation over stable ground, defined by the swissTLM3D land surface classification. The reconstructed time series provides geometric constraints to precisely model the preconditioning phase leading up to the May 2025 Nesthorn-Birchglacier hazard cascade, which may help mitigate future risks in mountainous terrain (see Jacquemart et al. 2026 in GM3.1)

How to cite: Knuth, F., Hodel, E., Heisig, H., Marty, M., Jacquemart, M., Bauder, A., Simmen, J.-L., and Farinotti, D.: Automated photogrammetric reconstruction of Birch Glacier, Switzerland (1946–2025): A high-density time series of topographic change preceding catastrophic glacier collapse, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22072, https://doi.org/10.5194/egusphere-egu26-22072, 2026.

The Southern Alps of New Zealand are regarded as an important key site for studying Holocene glacier chronologies in the mid-latitudinal southern hemisphere. Consequently, most global reviews of the topic include respective records and utilise them for (intra-)hemispheric correlations and palaeoclimatic analyses. These particular approaches are, however, closely connected to three common paradigms: (i) There is a representative and reliable compilation of glacier records for the entire Southern Alps, (ii) the European Alps are a well-suited and appropriate northern hemispheric glacier region for any comparative purpose, and (iii) air temperatures are the sole relevant driver of glacier variability in New Zealand.

In a recent study 10Be cosmogenic radionuclide dating (CRN) and Schmidt-hammer exposure-age dating (SHD) were applied to extent the regional database and obtain surface-exposure ages from moraines on Holocene glacier forelands in eastern Aoraki/Mt.Cook National Park, Arrowsmith Range, and Liebig Range. Re-calculated published 10Be CRN age data were, alongside previously obtained results from both central Aoraki/Mt.Cook and Westland/Tai Poutini National Parks, utilised for a comparative chronological analysis. Unlike previous approaches glacier records were differentiated by sub-regions of the Southern Alps and interpreted accordingly. Neither amalgamation of individual glacier records nor non-differentiated compilation took place. This multi-proxy approach was combined with detailed geomorphological mapping and assessment to tackle the regionally specific 'geomorphological uncertainty' potentially interfering with all subsequent interpretation of chronological data.

Chronological analysis and subsequent palaeoclimatic interpretation worked well if they were restricted to sub-regional levels. In the Arrowsmith Range strong glacial activity and multiple advances during the Early Holocene could be confirmed, with a similar pattern likely for the Liebig Range. A correspondence to frequent Early Holocene cold periods indicated by rock glacier activity in the Ben Ohau Range is obvious. But in contrast to these drier eastern sub-regions no evidence for Early Holocene advances exists for central and western sub-regions. At Classen Glacier in eastern Aoraki/Mt.Cook National Park, geomorphologically reliable morainic evidence shows a significant Mid-Holocene advance at c. 5.4 ka. It is possibly corresponding to evidence from Mueller and Tasman Glaciers. This advance coincides with an intensification of westerly airflow established around that time. Together with a 'Little Ice Age'-maximum during the mid-/late 18th century CE in Aoraki/Mt.Cook National Park and recent advances at the end of the 20th century it also indicates that (seasonal) atmospheric circulation patterns, in particular the intensity of westerly airflow, and precipitation should not be ignored as climatic factors influencing glacier variability. Finally, with its pronounced West-East precipitation gradient potentially responsible for different sub-regional glacier records, the Southern Alps share several glaciologically relevant climatic conditions with the maritime Scandinavian Mountains, but hardly with the generally drier European Alps.

Further refinement of the Holocene glacier history for the Southern Alps constitutes a significant challenge. It requires a more detailed understanding of both the variability of individual glacier records and the need for spatial differentiation before attempting to compile a representative Holocene glacier chronology for the entire Southern Alps. Furthermore, certain common paradigms need to be critically reviewed and re-considered. 

How to cite: Winkler, S.: Re-visiting New Zealand's Holocene glacier chronology - Time to overcome certain paradigms and consider spatial differentiation?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1403, https://doi.org/10.5194/egusphere-egu26-1403, 2026.

EGU26-2778 | Posters on site | GM9.2

Late Quaternary paraglacial and periglacial deposits in the high mountains of Taiwan 

Margot Böse and Robert Hebenstreit

During the last Pleistocene glacial cycle, Taiwan's high mountain ranges were glaciated in the uppermost altitudinal zone with a calculated lowering of the equilibrium line altitude (ELA) of ca. 1500 m down to 2800 m (Hebenstreit et al. 2025). Glacial erosion of the upper valley reaches formed trough-valleys. Lateral and terminal moraines as well as outwash deposits were deposited at or near the ice margins, respectively, at different stages of the glaciation. Subsequently, slope processes and fluvial activity have been reworking those sediments and reshaping those landforms during and after the glaciation to adjust the relief gradually to its present shape. These processes are called paraglacial processes (Ballantyne 2002).

 

In the Hsueh Shan range, we mapped a sequence of terraces composed of cobbles and boulders at the confluence of the Taoshan river and the Chijiawan river at an altitude of ca. 1900 m, which corresponds with the assumed lowest altitude of the last-glacial glacier termini. Surface exposure dating with paired in-situ produced terrestrial cosmogenic nuclides (TCN) of meter-sized boulders on the terrace surfaces gives evidence of enhanced glacio-fluvial activity, presumably reworking glacial deposits during the last phase of the glaciation at the Pleistocene-Holocene transition. 

 

Lowering of the altitudinal zones and consequently of surface processes during glacial times entails periglacial processes on slopes not affected by glacial or fluvial processes (Böse 2006). This includes frost weathering and solifluction. The periglacial zone is presently restricted to altitudes above 3500 m in Taiwan.

 

A sediment profile at ca. 2050 m on the slope above the glacio-fluvial terraces shows a stratification typical for cover beds in mountainous periglacial environments (Kleber & Terhorst 2024): Above debris of local underlying bedrock follow layers enriched by aeolian dust. The sediment has been partly reworked and mixed by solifluction. Optically stimulated luminescence (OSL) ages of the silty matrix confirm its formation during the last glacial cycle; and a lowering of the periglacial altitudinal zone of 1500 m can be inferred.

 

References

Ballantyne, C. K., 2002: Paraglacial geomorphology. Quaternary Science Reviews

21 (18–19), 1935-2017.

 

Böse, M., 2006: Geomorphic altitudinal zonation of the high mountains of Taiwan. Quaternary International 147 (1), 55-61.

 

Hebenstreit, R., Hardt, J., Böse, M., 2025: The lowermost last‐glacial equilibrium line altitude in the Taiwanese Central Mountain Range and its implications for the palaeoclimate and the tropospheric moisture transport in East Asia. Journal of Quaternary Science 40 (5), 831-846.

 

Kleber, A., Terhorst, B. (eds.) 2024: Mid-Latitude Slope Deposits (Cover Beds)

2nd Edition. Elsevier Science

How to cite: Böse, M. and Hebenstreit, R.: Late Quaternary paraglacial and periglacial deposits in the high mountains of Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2778, https://doi.org/10.5194/egusphere-egu26-2778, 2026.

EGU26-5367 | ECS | Orals | GM9.2

Lateglacial glaciers dynamics in the Mont Blanc foreland (Northern French Alps): new chronological and geomorphological constraints, with model-data coupling in the Arve Valley 

Quentin Portal, Christian Crouzet, Jean-François Buoncristiani, Tancrède Leger, Guillaume Jouvet, and Julien Carcaillet

Despite several studies (Coutterand, 2010 and references theirin) over the past decades, the chronology of glaciers advance and expansion at the Last Glacial Maximum (LGM) and subsequent retreat during the Lateglacial period in the northern French Alps remains poorly constraint, as data are still too scarce and sometimes contradictory. In this area, the interactions between major glaciers, such as the Rhône and Arve glaciers in the north and Isère glacier in the south, represent major challenges for reconstructing post-LGM glacial dynamics. Here, we present a new framework for understanding Lateglacial glacial dynamics in the Arve Valley, integrating 18 new 10Be exposure ages from glacially-transported boulders, with revised geomorphological mapping based on LiDAR-derived DEMs.

Our results indicate that the deglaciation of the Arve Valley initiated with a phase of glacial thinning around 17.6 ka BP. The Arve glacier subsequently thinned progressively but persisted in the downstream sector of the valley until the end of a readvance phase at 15.9 ka BP. Then, the glacier retreated by over 30 km within 300 years, before withdrawing toward the Mont-Blanc massif ahead of the Younger Dryas readvance.

These findings are integrated with previous studies (Wirsig et al., 2016; Roattino et al., 2022; Serra et al., 2022) conducted in the Northwestern Alps, including the Lyon piedmont lobe and the Mont-Blanc massif area, to propose a regionally consistent deglaciation scenario. To further refine our understanding, we confront 10Be exposure ages with numerical simulations using the Instructed Glacier Model (IGM, Leger et al., 2025). A dual approach enables a critically assessment of both methods: calibration of exposure ages corrections (e.g., erosion rates, snow shielding) using a model run, and inversely, using calculated exposure ages to constrain the resulting model. This will enable us to analyse possible deglaciation rates and spatial patterns in the Northwestern Alps, as well as the influence of key parameters such as geography, topography, and climate.

Coutterand, S. 2010: Etude géomorphologique des flux glaciaires dans les Alpes nord-occidentales au Pléistocène récent : du maximum de la dernière glaciation aux premières étapes de la déglaciation. PhD thesis. Université Savoie Mont-Blanc.

Leger, T. P. M., Jouvet, G., Kamleitner, S., Mey, J., Herman, F., Finley, B. D., Ivy-Ochs, S., Vieli, A., Henz, A. & Nussbaumer, S. U. 2025: A data-consistent model of the last glaciation in the Alps achieved with physics-driven AI. Nature Communications 16, 848. https://doi.org/10.1038/s41467-025-56168-3.

Roattino, T., Crouzet, C., Vassallo, R., Buoncristiani, J.-F., Carcaillet, J., Gribenski, N. & Valla, P. G. 2022: Paleogeographical reconstruction of the western French Alps foreland during the last glacial maximum using cosmogenic exposure dating. Quaternary Research 111, 68–83. https://doi.org/10.1017/qua.2022.25.

Serra, E., Valla, P. G., Gribenski, N., Carcaillet, J. & Deline, P. 2022: Post-LGM glacial and geomorphic evolution of the Dora Baltea valley (western Italian Alps). Quaternary Science Reviews 282, 107446. https://doi.org/10.1016/j.quascirev.2022.107446.

Wirsig, C., Zasadni, J., Christl, M., Akçar, N. & Ivy-Ochs, S. 2016: Dating the onset of LGM ice surface lowering in the High Alps. Quaternary Science Reviews 143, 37–50. https://doi.org/10.1016/j.quascirev.2016.05.001.

How to cite: Portal, Q., Crouzet, C., Buoncristiani, J.-F., Leger, T., Jouvet, G., and Carcaillet, J.: Lateglacial glaciers dynamics in the Mont Blanc foreland (Northern French Alps): new chronological and geomorphological constraints, with model-data coupling in the Arve Valley, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5367, https://doi.org/10.5194/egusphere-egu26-5367, 2026.

EGU26-5511 | ECS | Posters on site | GM9.2

Freeze-thaw cycles investigate weathering properties of different lithologies used in 10Be exposure age dating in the Eastern Alps 

Gerit E.U. Griesmeier, Andreas Hausenberger, Cosmin Nacu, Jürgen M. Reitner, Sandra Braumann, Stephanie Neuhuber, and Daniel P Le Heron

During the Last Glacial Maximum (LGM), many glaciers in the Eastern Alps terminated in narrow inneralpine valleys resulting in a limited amount of datable landforms. At the former Enns and Mur Glaciers, boulders, at or close to laterofrontal moraine ridges were dated with cosmogenic 10Be. Boulders at the Mur Glacier are composed of weathering-resistant pegmatite gneiss, whereas quartzbreccia/greywacke was the only suitable boulder lithology in the Enns Glacier region. This lithology consists of large quartz components within a fine matrix and is more easily affected by weathering. Ages inferred from 10Be concentrations in pegmatite gneisses (Mur Glacier) are around 20 ka, in accordance with other ages around the Alps. In contrast, Enns Glacier boulders yielded surprisingly young ages between 14-17 ka. In order to obtain plausible LGM ages via erosion corrections from the 10Be concentrations, a 30 cm thick surface layer would need to be removed (if the boulder was at the surface since deposition). In order to understand, if such a large amount of material can be removed from the quartzbreccia, we applied freeze-thaw cycle experiments to both lithologies. For the experiment, we produced four cubes, roughly 2x2x4 cm in size, three of quartzbreccia and one of pegmatite gneiss. Each of the quartzbreccia cubes has a different thickness of weathering crust (0-4 cm) with abundant holes and cracks. Their mineralogical composition is quartz, carbonate, and phyllosilicates with a preferential orientation. All cubes were dried, weighted and their volume determined and afterwards they were subjected to over 100 freeze-thaw cycles. To simulate moisture and rain, the cubes were thawed in a water bath at a constant temperature of 20 °C.  All cubes were photodocumented before the test, roughly every three weeks over a 4 months period, and after the test. CT scans were made of one quartzbreccia cube before and after the test to better visualise structural changes within the cube. The freeze-thaw cycles show that the quartzbreccia cubes weather much more intense than the pegmatite gneiss. No visual changes were detected in the latter, whereas quartzbreccia cubes constantly changed. Water seems to enter the cubes following pathways along the aligned sheet silicates. These delicate minerals are then destroyed and once enough matrix is removed, larger quartz crystals fall out, which is nicely seen on the photos. Overall, this process seems to result in a rather continuous loss of material, but varies in different cubes and even on different planes of the cubes. As a result, cosmogenic 10Be is removed constantly. Additionally, the nature of discontinuous weathering results in an inhomogeneous 10Be production due to edge effects resulting in loss of 10Be at the rim of a raised quartz pebble. In summary, the freeze-thaw cycles show that the quartzbreccia weathers much faster than the pegmatite gneiss and therefore the age difference could at least partly be explained. Therefore, caution is required when dating conglomerates, breccias or similar lithologies with cosmogenic 10Be.

How to cite: Griesmeier, G. E. U., Hausenberger, A., Nacu, C., Reitner, J. M., Braumann, S., Neuhuber, S., and Le Heron, D. P.: Freeze-thaw cycles investigate weathering properties of different lithologies used in 10Be exposure age dating in the Eastern Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5511, https://doi.org/10.5194/egusphere-egu26-5511, 2026.

A detailed morphometric and modelling-based analysis was conducted on 197 palaeocirques across the western Putorana Plateau, Central Siberia, to refine reconstructions of mountain glacier extent and associated palaeoclimatic conditions during the last major phase of glaciation. Previous work in the region quantified cirque geometry and inferred palaeo-equilibrium line altitudes from cirque floor elevations. Here, these geomorphological constraints are integrated with physically based glacier reconstructions using the PalaeoIce 2.0 model to simulate ice thickness, surface geometry, and glacier extent for individual cirques.

The cirques display mean widths of approximately 1000 m and mean lengths of 936 m, forming near-circular, amphitheatre-like landforms indicative of sustained glacial erosion. Cirque heights range from 111 to 591 m, reflecting both variability in erosional intensity and topographic controls. Strong positive correlations between length, width, and height (L×W: 0.758; L×H: 0.610) indicate proportional scaling of cirque dimensions. Mean cirque slopes are 23.5°, with steep headwalls reaching up to 80°, while more than half of cirque areas are characterised by gentler slopes associated with overdeepened floors, where tarns are frequently present.

Cirque floor altitudes range from 447 to 1568 m, providing first-order constraints on former glacier geometry. PalaeoIce 2.0 reconstructions indicate a mean palaeo-equilibrium line altitude of approximately 658 m, corresponding to a depression of ~1042 m relative to present conditions. Modelled glacier geometries are consistent with extensive, topographically confined mountain glaciers developed within individual cirques during the Last Glacial Maximum. Associated palaeoclimate estimates suggest mean summer air temperatures of approximately −1.5 °C and annual precipitation of ~634 mm to sustain such glaciation.

These results demonstrate the value of combining cirque morphometrics with numerical ice-flow modelling to refine palaeoglacier reconstructions in high-latitude mountain regions. The PalaeoIce 2.0 simulations provide an independent, physically based framework for evaluating cirque-derived palaeoclimate inferences and for improving understanding of mountain glacier behaviour along the margins of larger ice-sheet systems.

How to cite: Oien, R. and Lee, E.: Integrating cirque morphometrics and numerical modelling reconstructions in Putorana, Central Siberia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10021, https://doi.org/10.5194/egusphere-egu26-10021, 2026.

EGU26-11933 | ECS | Posters on site | GM9.2

Reconstructing the Quaternary glaciation of the central European uplands and its palaeoclimate implications 

Cristina I. Balaban, Marco Nieslony, David Krause, Zbyněk Engel, Marek Křížek, Julien Seguinot, Harry Zekollari, and Martin Margold

During the Pleistocene ice ages, Central Europe formed a mostly unglaciated corridor between the Fennoscandian Ice Sheet and the Alpine ice complex. The mountains of this region hosted small ice masses at the time. However, the extent, timing and climate conditions under which glaciers existed, as well as their erosional imprint on the landscape remain poorly understood. Solving these challenges is important for understanding the impact glaciation may have had on the distribution of biota and permafrost, which, in turn, can be used to reconstruct former human migration routes in Central Europe. This project aims to reconstruct the past glaciation of the Central European uplands and its palaeoclimate implications, focusing on the mid-elevation mountains in the region, such as the Bohemian/Bavarian Forest, the Fichtel Mountains, the Ore Mountains, and the Sudetes.

Firstly, we aim to identify and date former ice extents and determine the style of glaciation through geomorphological mapping of glacial depositional and erosional landforms and their radiometric dating with terrestrial cosmogenic nuclides and optically stimulated luminescence. Secondly, we will conduct morphometric analyses and geophysical surveys to determine the degree of glacial erosion of cirques and valleys and assess the influence of plateau surfaces as potential snow or ice accumulation areas. Finally, we will apply a numerical glacier model (Parallel Ice Sheet Model) to identify the degree of temperature cooling and precipitation increase or decrease from present-day to grow glaciers that match the mapped and dated extents. Thus, an understanding of past glaciation and climate over Central Europe during the Pleistocene will be produced, with a wide relevance for the palaeoclimatology, ecology, and archaeology research communities. This poster will introduce the project and present initial results.

How to cite: Balaban, C. I., Nieslony, M., Krause, D., Engel, Z., Křížek, M., Seguinot, J., Zekollari, H., and Margold, M.: Reconstructing the Quaternary glaciation of the central European uplands and its palaeoclimate implications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11933, https://doi.org/10.5194/egusphere-egu26-11933, 2026.

EGU26-12599 | ECS | Orals | GM9.2

Quantifying topoclimatic control on glacier Equilibrium Line Altitudes at the regional and global scale 

Lukas Rettig, Matthias Huss, and Marin Kneib

Reconstructions of glacier Equilibrium Line Altitudes (ELAs) from geomorphological evidence are often the only source of quantitative palaeoclimatic information in mountainous regions. The ELA is the average altitude of zero net mass balance and divides a glacier into an accumulation and an ablation area. While primarily controlled by summer temperature and winter precipitation, the position of the ELA is also frequently modulated by local topoclimatic factors, such as shading, supraglacial debris cover, avalanching or wind-driven snow redistribution. As a result, there can be substantial differences of several 100 meters between ELAs of neighbouring glaciers within the same climatic region. If such topoclimatic controls are not accounted for, this can introduce notable biases into ELA-based palaeoclimate reconstructions.

To better constrain the effect of topoclimatic control on glacier ELAs at the regional to global scale, we present the results of a comprehensive data analysis based on the Randolph Glacier Inventory (RGI), version 7.0. We compare glacier-specific ELAs calculated through the Accumulation Area Ratio and Area-Altitude Balance Ratio methods to a variety of topographic parameters, such as the amount of received solar radiation, the curvature of the ice surface and the topographic openness of the terrain. We show that there is a strong correlation between local ELA differences and some of these parameters and use a machine-learning tool to predict this ELA offset using only a digital elevation model and a glacier outline as input. This tool can be used to assess the topographic bias related to any calculated ELA and has the potential to lead to more reliable palaeoclimate reconstructions in a variety of settings.

How to cite: Rettig, L., Huss, M., and Kneib, M.: Quantifying topoclimatic control on glacier Equilibrium Line Altitudes at the regional and global scale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12599, https://doi.org/10.5194/egusphere-egu26-12599, 2026.

EGU26-13373 | Posters on site | GM9.2

A new low-latitude, high-elevation cosmogenic beryllium-10 production rate from the Rwenzori Mountains, Uganda 

Margaret Jackson, Nathan Anderson, Meredith Kelly, James Russell, Andrea Mason, Sloane Garelick, Alice Doughty, Bob Nakileza, Laura Hutchinson, George Geier, and Alan Hidy

Cosmogenic nuclide surface-exposure dating has emerged as a key tool in glacial geomorphology. Accurate application of the technique relies first on establishing local nuclide production rates using independently dated calibration sites. Certain regions of the world, such as the low latitudes, host few existing calibration sites. Developing local production rate calibrations in the low-latitudes is therefore a crucial first step for robust application of surface-exposure dating in these regions, particularly as cosmogenic nuclide production is theoretically more sensitive to changes in Earth’s magnetic field in the low-latitudes. Here we present a new local cosmogenic beryllium-10 production rate from the equatorial Rwenzori Mountains of Uganda based on radiocarbon dating of basal sediments from the moraine-dammed Lake Mahoma (~21.3 kyr BP; ~2,900 m asl). We also present the results of a systematic investigation of the performance of different parameters used to scale production rates spatially and temporally (e.g., scaling frameworks, geomagnetic field reconstructions, atmospheric models) using two public online calculators and limiting radiocarbon age data from nearby Lake Kopello (~4,000 m asl) in the Rwenzori. Our results highlight the sensitivity of low-latitude, high-elevation cosmogenic nuclide production to discrete parameters and underline the need for additional low-latitude production rate calibration sites.

How to cite: Jackson, M., Anderson, N., Kelly, M., Russell, J., Mason, A., Garelick, S., Doughty, A., Nakileza, B., Hutchinson, L., Geier, G., and Hidy, A.: A new low-latitude, high-elevation cosmogenic beryllium-10 production rate from the Rwenzori Mountains, Uganda, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13373, https://doi.org/10.5194/egusphere-egu26-13373, 2026.

EGU26-13791 | Orals | GM9.2

Examining the nature and timing of deglaciation in Britain: new evidence from the Arenigs, Brecon Beacons and South Wales Valleys 

Philip Hughes, Oliver Thomas, Christopher Darvill, Peter Ryan, and David Fink

New 10Be exposure ages from the Arenig mountains, North Wales have been obtained to complement 36Cl ages and help constrain the timing of deglaciation in NE Wales. The last phase of cirque glaciation is dated to the Younger Dryas and this is consistent with previous assumptions of deglaciation in Wales. In South Wales, in the Brecon Beacons, the last cirque glaciers were higher than those in the north, which is consistent with increasing cirque altitude with lower latitude. Radiocarbon dating from bogs inside of moraines in these cirques also supports a Younger Dryas age for the last phase of glaciation. However, further south in the South Wales Valleys, the last former cirque glaciers were at some of the lowest altitudes in Wales. The glaciers occupied cirques that are lower than in the nearby Brecon Beacons and these cirques represent an anomalous population of low-lying cirques compared with the rest of Wales. Reasons for this are either because 1) wetter conditions existed the South Wales Valleys than the rest of Wales leading to lower cirque glaciation during the Younger or 2) the last cirque glaciers were present and formed moraines prior to the Younger Dryas, possibly when the Welsh Ice cap covered Wales north of the Brecon Beacon watershed divide. Ongoing work will apply 10Be exposure dating from moraine boulders and 14C dating from bogs inside of moraines in the cirques of the Brecon Beacons and South Wales Valleys to test these hypotheses further. 

How to cite: Hughes, P., Thomas, O., Darvill, C., Ryan, P., and Fink, D.: Examining the nature and timing of deglaciation in Britain: new evidence from the Arenigs, Brecon Beacons and South Wales Valleys, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13791, https://doi.org/10.5194/egusphere-egu26-13791, 2026.

EGU26-14454 | Orals | GM9.2

A multiproxy speleothem-based approach to reconstructing alpine glaciation beyond the limits of geomorphological evidence 

Jonathan Baker, Alexandre Honiat, Peter Wynn, Gina Moseley, Regina Mertz, and Christoph Spötl

The sensitivity of alpine glaciation to climatic warming is underscored by global reductions in ice mass over the last century and accelerated losses observed in recent decades. Given the dependence of local populations, infrastructure, and ecosystems on reliable snowpack and meltwater supply, the forecasted demise of many mountain glaciers critically motivates investigations into the dynamics underlying glacial retreat and advance under past boundary conditions. However, the timing and extent of glacial limits are progressively less well constrained through geologic time, particularly in mountain regions, due to the inevitable loss of geomorphic indicators through subsequent glacial advance and erosion. Secondary mineral deposits in some alpine caves offer a unique solution to glacial reconstructions, because warm-based ice cover allows the cave system to remain unfrozen with active speleothem growth. Importantly, the loss of soil cover and presence of glacial ice induces an abrupt switch from a carbonic-acid to a sulfuric-acid dominated system in caves hosted by impure carbonate rocks, which can be detected through geochemical analysis of radiometrically dated speleothems. While this category of ‘subglacial speleothems’ has long been described, only recently has a thorough multiproxy approach been developed and tested, which can robustly identify the timing and dynamics of glaciation over alpine cave sites. In addition to key changes in the stable-isotope composition of carbon (δ13C) and oxygen (δ18O), the dominance of sulfuric-acid dissolution leads to an increase in speleothem sulfate, often by more than an order of magnitude, which may be accompanied by a decrease in the δ34S of sulfate due to enhanced sulfide oxidation. Glacial weathering processes are captured by certain trace elements in speleothem calcite, whereas the redox evolution of infiltrating waters (reflecting the hydrological balance of surface and subglacial meltwaters) is reflected in the oxygen-isotope composition of speleothem sulfate. Finally, U-series dating (U-Th and U-Pb) allows for accurate geochronological constraints, sometimes with per mil precision, throughout the Quaternary and beyond. Herein, we present case studies from the European Alps and Western Caucasus that successfully document the advance and retreat of warm-based glaciers without reference to surficial deposits and landforms. We further discuss uncertainties associated with the site-specific behavior of geochemical proxies that may limit their application to some glacial reconstructions.

How to cite: Baker, J., Honiat, A., Wynn, P., Moseley, G., Mertz, R., and Spötl, C.: A multiproxy speleothem-based approach to reconstructing alpine glaciation beyond the limits of geomorphological evidence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14454, https://doi.org/10.5194/egusphere-egu26-14454, 2026.

EGU26-14826 | Posters on site | GM9.2

Distal Cirque Contribution to the Northern Cordilleran Ice Sheet, Yukon Territory  

Brent Ward, Derek Cronmiller, Jessi Steinke, Jeffery Bond, and Michel Lamothe

Yukon Territory has been repeatedly affected by the northern Cordilleran Ice Sheet (NCIS). Although termed an ice sheet, it is better described as an ice complex, with quasi-independent lobes originating from mountainous areas around the border of the Yukon. This ice complex produced irregular, digitate glacial limits largely on the plateau area of central Yukon, at the eastern edge of unglaciated Beringia. These limits have broadly followed a pattern of progressively diminished extent. It is likely that variable precipitation across the source areas of these lobes affected their extent and timing during various glacial cycles. The growth model of the NCIS is contingent on ice from numerous cirques and ice fields in the source areas eventually amalgamating into these large, coalescent, ice lobes. What is unclear is the contribution of cirque and valley glaciers from the distal mountainous areas near the limits of glaciation. This research describes the contribution of cirque and valley glaciers in two areas at or near the limit of glaciation from MIS 6-2.

 

Ruby Range in southwest Yukon was affected by the Saint Elias lobe. It encompasses the limits of MIS 2, 4 and 6 glaciations. Stratigraphic analysis paired with 10Be surface exposure dating indicates extensive local ice production from cirques and plateau surfaces during MIS 2. During early MIS 2, local valley glaciers advance to the edge of the range but had retreated up valley during inundation by the St. Elias lobe, likely due to local precipitation reduction. These alpine ice centres were responsive to deglacial climatic fluctuations and hosted significant re-advances during the Older Dryas during rapid retreat of the St. Elias Lobe despite their location in the rain shadow of the St. Elias Mountains. The MIS 4 limit is slightly more extensive than the MIS 6 limit, likely because local ice growth contributed significantly to this portion of the St. Elias Lobe. The record and limit of the MIS 6 glaciation is poorly constrained here but 150 km to the NW, MIS 6 is 4 km more extensive than 4.

 

Granite Creek is in Gustavus Range in central Yukon at the MIS 2 limit of the Selwyn lobe. It was completely overrun during MIS 6, but cirque glaciers were extensive early enough that the Selwyn lobe did not inundate local cirque valleys. Stratigraphic studies indicate extensive MIS 4 cirque glaciation but provide no evidence of a proximal Selwyn lobe. During MIS 2, cirque glaciers near the margin were partially overrun by the Selwyn lobe. A tongue of the Selwyn lobe blocked Granite Creek forming a lake, and cirque glaciers terminating in the lake advanced due to floating ice margins. These limits are not reflected in the geomorphic record; well-defined MIS 2 moraines are recessional from this maximum.

 

This research indicates peripheral ice accumulation could contribute to the NCIS. However, stratigraphic studies indicate that peripheral ice sources in many cases were asynchronous with advances from primary source areas, likely due to variations in precipitation caused by the expansion of the CIS.

 

How to cite: Ward, B., Cronmiller, D., Steinke, J., Bond, J., and Lamothe, M.: Distal Cirque Contribution to the Northern Cordilleran Ice Sheet, Yukon Territory , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14826, https://doi.org/10.5194/egusphere-egu26-14826, 2026.

EGU26-16061 | ECS | Orals | GM9.2

Glacial record and 36Cl cosmogenic dating in the Nevados de Chillán Volcanic Complex, Northern Patagonia 

Sofía Navas, Alfonso Fernández, Edilia Jaque, Lewis Owen, Paula Figueiredo, and Nathan Stansell

Andean landscapes contain key paleoclimate records of the Southern Hemisphere. However, many mountain regions in the Andes remain scarcely investigated in detail. In this study, we present an analysis of the Nevados de Chillán Volcanic Complex (NCVC), in Southern Chile (37ºS), aiming at unveiling the potential of this landscape to register past climatic conditions. This site is within a region of Temperate-Mediterranean climate transition (TMT; 35.5°–39.5°S), which comprises most of the Southern Volcanic zone (SVZ) of the Andes, that host the most active volcanoes of the cordillera, almost all of them are ice-capped. These volcanoes witnessed the multiple expansions and retreats of the Patagonian Ice Sheet (PIS) during Pleistocene glaciations and of smaller mountain glaciers during the Holocene, reflecting local climatic variations. Our findings show the NCVC preserves a recent and diverse glacial record, as identified with a detailed geomorphological mapping (1:20.000). The elevation and preservation of glacial deposits and scoured bedrock point to multiple glacial advances after the Last Glacial Maximum. Current analysis of ages obtained with 36Cl dating of andesitic boulders atop moraines support field observations and geomorphological interpretations, with different episodes from Early-Middle Holocene until the last centuries. The oldest measurements in could represent late glacial advances, which also occurred in central Andes and Patagonia. Ages from frontal moraines are coeval with the Little Ice Age, consistent with results of recent studies in adjacent volcanic areas. From lateral moraines dispersed age results suggest persistent glacial activity since the last millennia until 200 years ago. The younger ages are supported by historical accounts from 19th century that document glacial extent comparable with the location of sampled boulders.  Overall, these results should be interpreted in light of uncertainties related to geomorphological mapping and especially with chronological constraints.  Despite these limitations, the integrated approach adopted here provides a useful framework to identify regional-scale patterns of glacier fluctuations and to assess their sensitivity to climatic variability during the Late Pleistocene–Holocene.

How to cite: Navas, S., Fernández, A., Jaque, E., Owen, L., Figueiredo, P., and Stansell, N.: Glacial record and 36Cl cosmogenic dating in the Nevados de Chillán Volcanic Complex, Northern Patagonia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16061, https://doi.org/10.5194/egusphere-egu26-16061, 2026.

EGU26-18100 | ECS | Posters on site | GM9.2

Towards Reconstructing Ice-Dynamical Holocene Glacier Fluctuations  

Marijke Van Cappellen and Harry Zekollari

Paleoclimatic evidence suggests that during the Holocene Climatic Optimum , glacier extent in many regions was substantially reduced or absent despite temperature conditions comparable to those observed today. This apparent discrepancy raises questions about the controls on glacier persistence over centennial to millennial timescales and the role of climate history, variability, and transient adjustment processes.  

In this work, we take first steps into investigating the evolution of glacier ice masses across the Holocene using a thermo-mechanical ice flow modelling framework. By exploring glacier response across key Holocene climate intervals, including periods of warming and cooling, we aim to examine how prior climate states, rates of change, and long-term disequilibrium may influence glacier extent under similar mean conditions. This approach provides a long-term context for present-day glacier evolution and offers insight into why modern glaciers may differ from their earlier Holocene counterparts under comparable climatic forcing. 

How to cite: Van Cappellen, M. and Zekollari, H.: Towards Reconstructing Ice-Dynamical Holocene Glacier Fluctuations , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18100, https://doi.org/10.5194/egusphere-egu26-18100, 2026.

Numerical models simulating potential future climate schemes are tested against different proxy-based reconstruction of paleoclimate and must be finely tuned. In the north Atlantic region, records indicate that the Last Glacial Termination was interrupted by rapid, high-amplitude reversals (Heinrich Stadial 1, Younger Dryas) during which temperatures got back to nearly ice-age cold conditions.
These events are thought to be year-round cooling periods and could be close analogues for future climate change in the north Atlantic region. Terrestrial glacial deposits give a high resolution vantage on abrupt shifts but remain poorly investigated. Previous studies based on surface exposure dating on glacial landforms show that glaciers retreats occurred within HS1 and YD, contradicting the prevailing models. Thus mapping palaeo-mountain glaciers former extend, dating their retreat and reconstructing their successive palaeo-equilibrium lines altitude allow to determine whether this pattern is a consensus for the northern hemisphere palaeo-glaciers. This approach also provides information on the timing and magnitude of past climate change. This study is based on the west coast of Ireland directly impacted by westerlies, located downwind of the North Atlantic Ocean and which contains key sites where palaeo-mountain glaciers let the footprints of their passage. Here, we present the first results  from the Geologic Perspectives on Abrupt Climate Change (GeoPAC2) project: Strengthening Ireland’s capacity for projecting future change. The new beryllium-10-dated glacier records reveals phase of ice retreat occurring within HS1. It questions the rising seasonality hypothesis which suggests an increase of summer temperatures during melting season. The results of this work will provide useful quantitative data for investigate North Atlantic climate variability and improve both climate and glaciological models.

How to cite: Roignot, A. and Bromley, G.: Palaeo-glaciers archives in western Ireland as a vantage on abrupt shifts of the Last Glacial Termination , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18404, https://doi.org/10.5194/egusphere-egu26-18404, 2026.

EGU26-18543 | ECS | Posters on site | GM9.2

Refining the history of changes in glacier geometry since the LIA at selected sites across the Austrian Alps  

Larissa von Römer, Harald Zandler, Lea Hartl, Marcela Violeta Lauria, Wolfgang Schöner, and Jakob Abermann

Information on past glacier states is fundamental for improving projections of future glacier evolution under ongoing climate change. In this study, we present a 170-years reconstruction of glacier area and volume changes of five glaciers providing comprehensive regional representation of the Austrian Alps, covering the period from the Little Ice Age (LIA) maximum (~1850) to the present. LIA glacier extents are derived from the national moraine-based LIA glacier inventory and complemented by historical topographic maps, terrestrial oblique photographs, historical orthophotos, and modern digital elevation models (DEMs) as references. 

We evaluate glacier geometry and its temporal changes at specific, data-constrained time points between the LIA maximum and the first comprehensive Austrian glacier inventory in 1969 by using monoplotting and DEM differencing techniques. Monoplotting intersects terrestrial photographs with DEMs to extract georeferenced glacier outlines from oblique photographs, for example. This approach allows us to derive glacier front variations or even approximate glacier areas at times where observational records are lacking. Historical DEMs were generated from scanned topographic maps, co-registered with modern elevation data, and used to compute volumetric changes. These multi-source datasets enable the reconstruction of glacier extents and ice-surface topography for several dates between the LIA and the first Austrian glacier inventory in 1969.  

Results show that, across all glaciers studied, area decline rates increased around the 1940s relative to the period between end of LIA (~1850) to the 1940s, coinciding with periods of positive summer air-temperature anomalies, particularly during the 1940s. Between approximately 1975 and 1990, decline rates decreased for most glaciers, reflecting the cooler period of the 1970s and 1980s. Whereas most glaciers stabilized or even temporary advanced around that period, Niederjochferner exhibited strong glacier area loss, consistent with front position measurements of the Austrian Alpine Club (Österreichischer Alpenverein, ÖAV). Relative area decline rates are generally larger for smaller glaciers. While the area of Gepatschferner, one of Austria’s largest glaciers, has decreased by around 30% since 1850, the medium-sized glaciers (< 6 km2 at LIA) have lost at least 45% of their LIA area. Despite its northward orientation, the Niederjochferner shows the strongest area reduction with over 70% since LIA. In contrast, the Mullwitzkees shows the lowest relative area retreat (≈45%) since LIA, even though it is the only southward facing glacier in this study. 

Ongoing work uses aerial imagery of high quality for its time, acquired by the US Army in 1945 covering the entire Austrian Alpine region, to reconstruct glacier extents and volumes. By generating orthophotos and DEMs, we aim to create a new national glacier inventory that can be used in various research fields. The extended time series of glacier volume and area change can provide valuable calibration and validation data for glacier models, such as the Integrated Glacier Model (IGM), enabling three-dimensional surface reconstruction and forward simulations under various climate scenarios.  

How to cite: von Römer, L., Zandler, H., Hartl, L., Lauria, M. V., Schöner, W., and Abermann, J.: Refining the history of changes in glacier geometry since the LIA at selected sites across the Austrian Alps , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18543, https://doi.org/10.5194/egusphere-egu26-18543, 2026.

EGU26-19769 | ECS | Orals | GM9.2

Validation Practices in Mountain Palaeoglacier Modelling 

Augusto C. Lima, Sjur Barndon, David M. Chandler, Li Yingkui, and Suzette G. A. Flantua

Numerical palaeoglacier modelling is being applied to mountain glacier systems worldwide to investigate past ice dynamics, climatic controls, and glacier–climate interactions.  At present, there is no overview or consensus framework for evaluating the performance of these models, nor agreed standards for determining whether simulated glacier distribution and geometry are plausibly reconstructed through time.

To assess how palaeoglacier models in mountains are being validated and evaluated, we conducted a systematic review of 94 coupled mass-balance–ice-dynamics palaeoglacier models worldwide. For each study, we recorded validation approaches (visual, quantitative, and/or statistical), the glaciological attributes evaluated (extent, area, ice thickness, mass balance, ice flow, glacier distribution), the validation datasets used (direct geomorphological evidence versus previous model outputs), and the spatial structure of validation (point-, line-, polygon-, or grid-based). We also synthesised validation workflows to document the datasets, metrics, and decision criteria employed.

Our results show that the methodological design used to validate model outputs vary considerably between studies. We found that 80% of reviewed studies incorporate visual evaluation of model outputs to some extent, and 43% rely exclusively on subjective visual interpretation. A further 4% of studies do not perform any form of model validation or evaluation. Most studies validate glacier length (89%), whereas 48% of cases validate only one individual model output. Geomorphic reconstructions are used as validation datasets in only 27% of studies, indicating that most validation workflows rely on mapped glacial landforms. Because glacier length and glacial landforms dominate validation strategies, point- and line-based features constitute the majority of spatial validation data, with polygon- or grid-based approaches remaining comparatively rare.

We observe that the interpretation of model performance often remains subjective and reliant on the judgement of a limited number of research authors, which hinders reproducibility and intercomparison across studies. This reliance on subjective visual interpretation reflects persistent challenges in palaeoglacier model validation that are not being solved by existing tools and workflows designed to measure model-data fit. Our review indicates that uneven geomorphic evidence coverage, positional uncertainty between mapped landforms and simulated ice margins, resolution mismatches between geomorphic data and model outputs, chronological dating uncertainties, parameter uncertainty, and ‘equifinality’ (i.e., where multiple parameter combinations can yield similarly plausible glacier geometries) within glacier models collectively hinder robust quantitative validation.

Therefore, we propose a probabilistic, equifinality-aware validation framework that integrates geomorphically based reconstructions, multiple model outputs (e.g., ice extent, ice thickness), temporal steps (e.g., LGM and present-day), and performance metrics (e.g., overestimation, underestimation). Our approach evaluates ice cover as a probability field derived from an ensemble of acceptable simulations, explicitly acknowledging parameter non-uniqueness of equifinal modelling outputs. This approach identifies spatial patterns of robust agreement and persistent uncertainty, avoids subjective selection of a best-fit simulation, and enables domain-wide validation that captures spatial and temporal heterogeneity in glacier behaviour, thereby providing a more transparent and reproducible basis for evaluating palaeoglacier model–data fit.

How to cite: Lima, A. C., Barndon, S., Chandler, D. M., Yingkui, L., and Flantua, S. G. A.: Validation Practices in Mountain Palaeoglacier Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19769, https://doi.org/10.5194/egusphere-egu26-19769, 2026.

EGU26-19840 | Posters on site | GM9.2

Interactions between trunk and local glaciers in distal Alpine valleys (southeastern Alps, Italy) 

Alessandro Fontana, Camilla Vidi, Giovanni Monegato, and Sandro Rossato

During the Last Glacial Maximum (LGM), the European Alps were occupied by an extensive glacial network in which major trunk glaciers interacted with smaller tributary glaciers. In several areas, local glaciers flowed in directions opposite to those of trunk glaciers, particularly in distal sectors characterized by complex topography and high precipitation. Despite their likely widespread occurrence, the dynamics, the peculiar morphologies and specific related depositional facies of these glacier–glacier interactions remain poorly constrained.

In the southeastern Alps (Italy), the glacial system was dominated by the Adige trunk glacier. Regional-scale reconstructions have defined glacier geometry, flow paths, and Equilibrium-Line Altitudes across the Adige and Astico valleys, including an ELA of ~1580 m for the Fiorentini glacier (Monegato et al., 2024). However, these reconstructions primarily address trunk glacier behavior, leaving the interactions with local valley glaciers largely unexplored.

This study focuses on valleys where the Adige trunk glacier interacted with local glaciers descending from adjacent massifs, with the two ice bodies flowing in opposite directionsunder conditions of high orographic precipitation. The Terragnolo Valley represents a key example, where the presence of the distal Adige glacier, is documented by moraines at elevations of ~1400 m a.s.l., and were it interacted with local glaciers descending from the Monte Pasubio massif (~2200 m a.s.l.). Similar geomorphological configurations are found also in the Vallarsa and Ossaria valleys, enabling a comparative, valley-scale analysis within the same glacial system.

In the Terragnolo Valley, the interaction zone is marked by a thick glacigenic succession extending for ~10 km upstream, dominated by locally derived carbonate clasts, with only minor contributions from lithologies typical of the trunk glacier. This sedimentary pattern indicates a complex interaction between the two ice bodies and raises key questions regarding ice-flow coupling, relative timing of glacier advances, and the degree of dynamic independence of local glaciers during the maximum extent of the trunk glacier.

Overall, the studied valleys highlight how interactions between trunk and local glaciers in distal sectors can generate complex dynamics and sedimentary architectures, providing new constraints for reconstructing Alpine glacier dynamics and the distribution of glacigenic deposits in the tributary valleys.

How to cite: Fontana, A., Vidi, C., Monegato, G., and Rossato, S.: Interactions between trunk and local glaciers in distal Alpine valleys (southeastern Alps, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19840, https://doi.org/10.5194/egusphere-egu26-19840, 2026.

EGU26-20278 | ECS | Orals | GM9.2

Are ice-contact lacustrine sediments in the Eastern Alps capable of constraining pre-LGM ice-stream network dynamics?  

Benjamin Spitaler, Alfred Gruber, Jürgen M. Reitner, and Michael C. Meyer

Mountain glaciers represent sensitive recorders of climate variability across a wide range of temporal and spatial scales. While their Lateglacial and Holocene dynamics are comparatively well constrained, glacier extent and behaviour prior to the Last Glacial Maximum (LGM) remain poorly documented in many mountain regions. In the Eastern Alps, the timing and magnitude of glacier advances during Marine Isotope Stage (MIS) 4 and MIS 3 are still debated, despite numerical glacier models predicting repeated pre-LGM advances into the Alpine foreland. This knowledge gap largely reflects (i) the scarcity of suitable terrestrial archives capable of recording such advances, (ii) the fact that organic material for radiocarbon dating is generally rare or absent in glacial settings and (iii) geomorphological evidence such as moraines is commonly eroded, reworked, or overprinted by subsequent glacier advances.

This study examines successions of ice-dammed glaciolacustrine sediments preserved in Alpine tributary valleys as alternative terrestrial archives for reconstructing pre-LGM glacier dynamics in the Eastern Alps. Ice-dammed lakes form when advancing trunk glaciers block the outlet of smaller tributary glaciers, creating temporary sediment traps that enable glaciolacustrine deposition. These ice-contact sediments record glacier advances and can survive multiple glacial cycles.

We focus on glaciolacustrine successions as ice-margin indicators and present a research approach that combines detailed sedimentological investigations with luminescence geochronology. The sedimentary architecture and stratigraphic relationships of ice-dammed sediments and associated delta complexes provide spatial constraints on an interconnected system of valley glaciers, including minimum ice-surface elevations and relative glacier extent. Chronological control is obtained using optically stimulated luminescence (OSL) and infrared stimulated luminescence (IRSL) dating of fine-grained quartz and feldspar (4–11 μm), respectively. Methodological challenges related to partial signal resetting are addressed using adapted bleaching-plateau tests [1], increasing confidence in the luminescence-based age constraints.

Our initial results from inneralpine sites indicate glacier advances which potentially reached into the Eastern Alpine foreland during MIS 4 and eventually MIS 3c, implying that glacier extent prior to the LGM was potentially more dynamic and spatially extensive than previously assumed. These results are consistent with numerical glacier model predictions [2].

From a methodological point of view, we conclude that (i) precise dating of ice-dammed lacustrine sediments enables reconstruction of the spatiotemporal dynamics of the associated ice-stream network, and (ii) luminescence-based lacustrine dating might complement geomorphological and cosmogenic-nuclide methods focused on lateral and frontal moraines used to delineate former ice margins.

 

References

1. Reimann, Tony; Notenboom, Paul D.; De Schipper, Matthieu A.; Wallinga, Jakob (2015): Testing for sufficient signal resetting during sediment transport using a polymineral multiple-signal luminescence approach. In: Quaternary Geochronology 25, S. 26–36. DOI: 10.1016/j.quageo.2014.09.002.

2. Jouvet, Guillaume; Cohen, Denis; Russo, Emmanuele; Buzan, Jonathan; Raible, Christoph C.; Haeberli, Wilfried et al. (2023): Coupled climate-glacier modelling of the last glaciation in the Alps. In: J. Glaciol. 69 (278), S. 1956–1970. DOI: 10.1017/jog.2023.74.

How to cite: Spitaler, B., Gruber, A., Reitner, J. M., and Meyer, M. C.: Are ice-contact lacustrine sediments in the Eastern Alps capable of constraining pre-LGM ice-stream network dynamics? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20278, https://doi.org/10.5194/egusphere-egu26-20278, 2026.

EGU26-21654 | ECS | Orals | GM9.2

Palaeoglaciations in the Polar and Subpolar Ural Mountains. 

Bartosz Kurjanski, Matteo Spagnolo, Irina Bushueva, Iestyn Barr, Brice Rea, Olga Solomina, and Stanislav Kutuzov

The Ural Mountains form a major physiographic boundary between the East European Plain and West Siberia, both repeatedly glaciated during the Pleistocene by the Barents–Kara ice sheet. Although the present-day topography reflects significant glacial modification, the extent, chronology, and interaction of mountain glaciers with the Barents–Kara ice sheet remain poorly constrained. Correlation of glacial and interglacial deposits across the range is hindered by incomplete sedimentary records, contrasting palaeoclimatic conditions, and limited chronological control, which collectively obscure regional glacial reconstructions.  This study presents an extensive mapping exercise of hundreds of moraines in the northern Urals. These landforms are then used to reconstruct palaeoglacier equilibrium line altitudes (ELAs) to assess glacier distribution and synchroneity of moraine formation. ELA trends along the Urals are analysed to evaluate whether, and where, montane ice caps developed during the last major glaciation. Furthermore, palaeo-ELA data are used to link former ice margins to dated moraines in the Polar Urals, providing new insights into the spatial and temporal dynamics of montane glaciations south of the Arctic Circle. The findings indicate that  the E-W asymmetry in the hypsometry of the Urals exerted  the primary control on the development of the piedmont glaciers on the lowlands. Furthermore, Glacier reconstructions combined with geomorphological evidence favour the existence of extensive montane ice caps over the Urals with moisture sourced from extensive ice dammed lakes  locates on both sides of the mountain range.

How to cite: Kurjanski, B., Spagnolo, M., Bushueva, I., Barr, I., Rea, B., Solomina, O., and Kutuzov, S.: Palaeoglaciations in the Polar and Subpolar Ural Mountains., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21654, https://doi.org/10.5194/egusphere-egu26-21654, 2026.

This study advances our understanding of Quaternary glaciation in the southeastern Tibetan Plateau by integrating geomorphic evidence with numerical ice sheet modeling to constrain paleoclimate and ice dynamics. We focus on the Haizishan Plateau, a key region with well-preserved landforms (cirques, U-shaped valleys, moraines) and cosmogenic nuclide chronology indicating major glaciations during MIS 2 and MIS 6. Using these geomorphic and chronological constraints, we first reconstructed the Last Glacial Maximum (LGM) ice margin and then applied the PaleoIce flowline model to estimate paleo-ice thickness and surface elevation. These independent geomorphic reconstructions were then compared to the results of three-dimensional paleo-ice sheet simulations performed with the Parallel Ice Sheet Model (PISM), which were driven by inferred paleoclimate conditions.

The PISM simulations indicate an LGM characterized by a temperature depression of ~4°C and precipitation levels 60–70% of modern values. The model successfully replicates the regional ice cap evolution, showing limited glacial extent during MIS 3 and restricted advances in MIS 4. Critically, the simulated ice configuration aligns well with the geomorphically reconstructed evidence, including glacial lineation patterns, landform zonation, and overall extent, validating the model's performance. Our findings demonstrate the power of combining geomorphic reconstruction with dynamical modeling to refine the glacial and climatic history of high-mountain regions.

How to cite: Fu, P. and Li, Y.: Modelling Haizishan paleo ice caps in the SE Tibetan Plateau during the last glaciation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21690, https://doi.org/10.5194/egusphere-egu26-21690, 2026.

CR2 – lce sheets, ice shelves and glaciers

The temporal evolution of near-surface ice slabs (> 1m thick) on the Greenland Ice Sheet (GrIS) has significant implications for understanding both past variability and future changes in ice sheet mass balance. These ice slabs, formed through the refreezing of meltwater in the firn layer, modulate surface runoff dynamics and affect the ice sheet’s meltwater retention capacity, which is critical for understanding future surface mass balance (SMB) sensitivity to climate change. With ongoing climate warming, the mechanisms driving the formation and expansion of these ice slabs are likely to intensify. There is a need for coupled SMB and sub-surface firn models that can effectively simulate near-surface firn and ice slab evolution, allowing us to predict their long-term impact on Greenland's contribution to global sea-level rise.

In this study we present a 1-D physically based model with high vertical resolution (1 cm) to simulate surface melt, percolation, refreezing, ice slab evolution, runoff, and surface mass balance (SMB) across the GrIS. The high vertical grid resolution facilitates continuous simulation of the evolution of ice layers with thicknesses ranging from 1 cm to several metres. We applied a novel, laboratory defined, temperature-dependent ice layer permeability criterion whereby all ice layers are permeable above –0.15 °C but become impermeable beyond 1 m thickness. The model incorporates a novel parameterization of vertical snow and firn compaction, replacing frequently used theoretical relationships derived for dry snow compaction with a laboratory-derived, viscosity-based relationship for refrozen snow / firn more commonly found within percolation zones.

We applied the model to the GrIS from 1999 to the end of the 21st century at a spatial resolution of 0.11° and a temporal resolution of 15 minutes. The simulations reproduce the observed distribution of past ice slab occurrences across the GrIS and generate near-surface firn density profiles and proglacial discharge hydrographs that closely match available field measurements. The model also captures the observed interannual variability in the runoff limit, demonstrating strong consistency with satellite-derived estimates. We forced the model with future climate projections to investigate the projected evolution of near-surface ice slabs and their implications for future vertical firn densification, meltwater runoff and surface mass balance.

How to cite: Laha, S. and Mair, D. W. F.: Temporal Evolution of Near-Surface Ice Slabs on the Greenland Ice Sheet: From Past Variability to Future Change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3362, https://doi.org/10.5194/egusphere-egu26-3362, 2026.

EGU26-3836 | Posters on site | CR2.1

Historical and Future Surface Mass Balance Contributions to Antarctic and Greenland Ice Sheet Freshwater Fluxes  

Kristiina Verro, Marte Hofsteenge, Charles Amory, Willem Jan van de Berg, Fredrik Boberg, Michiel van den Broeke, Matthias Carney, Elizabeth Case, Christiaan van Dalum, Xavier Fettweis, Nicolaj Hansen, Ruth Mottram, Martin Olesen, and Maurice van Tiggelen

Freshwater fluxes from the Antarctic and Greenland ice sheets play a critical role in sea-level rise, ocean circulation, and the global climate system. These fluxes arise from both dynamical processes—such as ice discharge, iceberg calving, and basal melting of ice shelves—and from surface mass balance processes. In Greenland, surface meltwater runoff is already a major contributor to freshwater input, and it is projected to become increasingly important in Antarctica as climate warming progresses. 

While regional climate models (RCMs) are key to studying climate at regional and local scales, relatively few are equipped with advanced snow and firn models capable of producing accurate surface mass balance results. Here, we present a comprehensive, state-of-the-art collection of regional climate model simulations (RACMO2, MAR, and HIRHAM5) for both Greenland and Antarctica, forced by historical and SSP-scenario CMIP6 Earth System Models and extending to the year 2100. We briefly assess the modelled surface mass balance, accumulation, melt, and runoff, and highlight aspects of atmosphere–snow/ice interactions that remain an active area of model development. This dataset can be used to prescribe freshwater fluxes from surface mass balance to oceanic or climate modelling experiments, or as a comparison against in situ observational datasets.

How to cite: Verro, K., Hofsteenge, M., Amory, C., van de Berg, W. J., Boberg, F., van den Broeke, M., Carney, M., Case, E., van Dalum, C., Fettweis, X., Hansen, N., Mottram, R., Olesen, M., and van Tiggelen, M.: Historical and Future Surface Mass Balance Contributions to Antarctic and Greenland Ice Sheet Freshwater Fluxes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3836, https://doi.org/10.5194/egusphere-egu26-3836, 2026.

EGU26-4980 | Posters on site | CR2.1

Viscosity of melt-affected snow/firn derived from laboratory-based uniaxial compression experiments. 

Douglas Mair, Grace Brown, and Sourav Laha

Enhanced climate warming across Arctic glaciers, ice caps and the Greenland Ice Sheet has intensified melt and refreezing processes, producing more widespread regions of melt-affected, near-surface (< 12 m depth) firn within accumulation areas. Accurately simulating this near-surface region is important, as it governs the evolving capacity of ice sheets to retain meltwater through refreezing and thus strongly influences surface mass balance. Although over short timescales (days to months) refreezing of meltwater dominates changes in the density of melt-affected firn, over longer timescales (decades to centuries), densification through vertical compaction of refrozen firn remains significant. Whilst there is a substantial body of both field and theoretical work addressing the issue of dry firn densification by compaction of snow into firn and ice, i.e. in the absence of melting and refreezing, there is a need for better understanding of densification by compaction in melt-affected snow / firn increasingly found across accumulation areas of ice sheets and glaciers.

 

Firn densification can be defined via a constitutive equation, calculating the vertical compression rate due to stress from the overburden pressure dependent on firn viscosity. Laboratory studies have demonstrated the potential of controlled experiments to constrain the viscosity of dry snow of varying densities.  However, similar experimental constraints do not yet exist for refrozen, melt-affected firn. In this study we extend such laboratory approaches to refrozen snow/firn to quantify their effective viscosities. We undertook confined uniaxial compression tests on snow/firn samples with known grain sizes and densities (c. 400 – 600 kg m-3), simulating expected ranges of overburden pressures to c. 12 m depth to establish the stress-strain rate relationships that define near-surface firn viscosities. Our experiments indicate an exponential increase in viscosity with density. The viscosity values calculated here for melt-affected snow/firn are broadly consistent with the lower envelope of viscosities reported in previous studies on cold dry firn, though they exceed those made in the field for temperate firn. The relationship of viscosity to snow/firn density allows our findings to be incorporated into large-scale firn densification and surface mass balance models, where resolving detailed microstructural processes and form is often impractical. By providing empirically constrained viscosity estimates tied directly to density, this work bridges a gap between field observations of melt-affected firn and the parameterizations required by regional and continental-scale models for more robust future projections of near-surface refreezing capacity of ice sheets and glaciers.

How to cite: Mair, D., Brown, G., and Laha, S.: Viscosity of melt-affected snow/firn derived from laboratory-based uniaxial compression experiments., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4980, https://doi.org/10.5194/egusphere-egu26-4980, 2026.

EGU26-6601 | Posters on site | CR2.1

Differing high-resolution Greenland ice sheet and peripheral ice caps surface mass balance since 1940 

Brice Noël, Xavier Fettweis, Willem Jan van de Berg, and Michiel van den Broeke

In the last decades, the Greenland ice sheet (GrIS) and its peripheral ice caps (GICs) have been rapidly losing mass through increased solid ice discharge and declining surface mass balance (SMB), i.e., the difference between precipitation accumulation and ablation from sublimation and surface runoff. Capturing SMB and its components at the local scale, notably across rapidly melting glaciers and ice caps, is therefore essential to accurately quantify Greenland’s contribution to global sea-level rise.

Here we compare long-term SMB reconstructions from two ERA5-forced regional climate models at ~5 km (MARv3.14 and RACMO2.3p2), further statistically downscaled to 500 m spatial resolution (1940-2024). These products are evaluated using in-situ measurements covering accumulation and ablation zones, as well as remotely sensed mass change records, showing good agreement. While the two models align Greenland-wide in terms of integrated SMB, individual components differ suggesting error compensation. MAR generally experiences both higher inland precipitation accumulation and larger surface runoff in marginal ablation zones than RACMO2, yielding approximately equivalent integrated SMB estimates. We examine these differences at the GrIS and GICs scale and further explore our products’ sensitivity to spatial resolution using corresponding downscaled SMB at 1 km.

How to cite: Noël, B., Fettweis, X., van de Berg, W. J., and van den Broeke, M.: Differing high-resolution Greenland ice sheet and peripheral ice caps surface mass balance since 1940, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6601, https://doi.org/10.5194/egusphere-egu26-6601, 2026.

EGU26-6842 | ECS | Posters on site | CR2.1

Observations of turbulent heat exchange, surface melt and refreezing on the Larsen C ice shelf, Antarctica (2022-2025) 

Maurice Van Tiggelen, Paul Smeets, Carleen Reijmer, and Michiel van den Broeke

Ice shelves currently stabilize the Antarctic ice sheet but are vulnerable to hydrofracturing in the future. A faster increase in surface melt compared to accumulation will cause a reduction in available firn pore space and will thus eventually lead to meltwater ponding at the surface.  However, current climate models disagree on the total volume of meltwater production and accumulation, and thus on the evolution of firn density over ice shelves. A lack of direct melt and refreezing observations on ice shelves, especially in areas of high melt, prevents a detailed benchmarking of climate and firn models.

Since 2022, a dedicated experiment takes place at two contrasting locations with existing long-term automatic weather observations on the Larsen C ice shelf, which is at risk of collapsing in the future. Here we present results from 3 years of data from an eddy covariance system, which measured the sensible and latent heat fluxes, a GNSS antenna that measured snow height change by interferometry (GNSSir), and a snow cosmic ray counter that measured the change in snow mass and thus bulk snow density.

We discuss the main challenges and recommendations in acquiring such data, the derived surface energy balance (SEB) fluxes, and the variation of bulk snow density due to accumulation and meltwater refreezing. We demonstrate that the turbulent fluxes can be correctly simulated with a bulk turbulence model, that the variation of surface roughness in time can also be extracted from GNSSir, and that the hourly melt fluxes and refreezing can be simulated within 10% accuracy using a skin energy balance model forced by standard single level observations.

How to cite: Van Tiggelen, M., Smeets, P., Reijmer, C., and van den Broeke, M.: Observations of turbulent heat exchange, surface melt and refreezing on the Larsen C ice shelf, Antarctica (2022-2025), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6842, https://doi.org/10.5194/egusphere-egu26-6842, 2026.

EGU26-7541 | ECS | Posters on site | CR2.1

Climate forcing time step requirements for firn modeling 

Tesse van den Aker, Peter Kuipers Munneke, Willem Jan van de Berg, Walter Immerzeel, and Michiel van den Broeke

The firn layer regulates how an ice sheet responds to climate change, by modifying how changes in surface temperature, snow accumulation and ablation affects the ice sheet mass balance.  The firn layer can be simulated with a firn densification model. However, a variety of climate forcing time steps have been used to force such firn models in literature, ranging from 3-hourly to daily, monthly, or even annually. Reasons for selecting certain climate forcing time steps are most often practical: the data are not available at smaller time steps, the amount of forcing data becomes too large, or computational resources are insufficient. Evaluation of the impact of the selected forcing time step is often absent or based on different lines of reasoning.

In this study, we force the firn model IMAU-FDM with different surface climate forcing time steps for the Antarctic Peninsula and southern Greenland Ice Sheet. We show that the modelled firn layer contains more pore space for larger forcing time steps. Locations with limited firn pore space due to seasonal melt are most sensitive.

The largest differences in modelled firn pore space arise when there is no diurnal cycle in the climate forcing input data. This allows for coexisting snowmelt and sub-zero surface temperatures, leading to immediate shallow refreezing of meltwater. We also found that parameterizations for e.g. fresh snow density can become unsuitable when applied outside the physical conditions or climate forcing time step on which they are based. We argue that (1) firn models require input with at least a sub-daily forcing time step, (2) use of parameterizations should be critically assessed and only used consistently with the way they were originally developed, and (3) the forcing time step should be considered when interpreting firn model output.

How to cite: van den Aker, T., Kuipers Munneke, P., van de Berg, W. J., Immerzeel, W., and van den Broeke, M.: Climate forcing time step requirements for firn modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7541, https://doi.org/10.5194/egusphere-egu26-7541, 2026.

EGU26-7895 | ECS | Orals | CR2.1

Emulating Greenland Ice Sheet melt and runoff from polar RCMs with machine learning 

Elke Schlager, Peter L. Langen, Ruth H. Mottram, Sebastian Scher, and Andreas P. Ahlstrøm

Accurate projections of ice sheet surface mass balance (SMB) are critical for sea-level rise estimates. Polar regional climate models (RCMs) coupled with firn models are the primary tools for simulating melt and projecting future SMB. However, the projections from different RCMs significantly deviate from each other. Additionally, the computational costs of polar RCMs and their firn models limit the creation of large ensembles needed to statistically assess the likely range in future melt and runoff.

Machine learning emulators offer a promising solution by enabling rapid predictions at a fraction of the computational cost. We therefore present machine learning emulators that predict daily surface melt and runoff from atmospheric variables from their associated polar RCM over Greenland. The emulators use a novel physics-informed, modular architecture that combines short-term weather patterns with long-term climate memory, capturing both immediate atmospheric forcing and accumulated firn characteristics.

Our work demonstrates that machine learning can successfully emulate firn model behavior from climate forcing alone. This represents a crucial first step toward computationally efficient emulation of polar RCMs, facilitating generation of large ensembles, sensitivity analysis, and potential integration as surrogate models within Earth system models.

How to cite: Schlager, E., Langen, P. L., Mottram, R. H., Scher, S., and Ahlstrøm, A. P.: Emulating Greenland Ice Sheet melt and runoff from polar RCMs with machine learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7895, https://doi.org/10.5194/egusphere-egu26-7895, 2026.

EGU26-8541 | Orals | CR2.1

Surface Elevation Changes and Mass Balance of the Greenland Ice Sheet from 2019 to 2024 from ICESat-2 Observations using a new MECEM model 

Rongxing Li, Mengfan Liu, Qiyuan Chen, Youquan He, Xiaofeng Wang, and Gang Qiao

As one of the main contributors of global sea level rise, the Greenland Ice Sheet (GrIS) has been experiencing significant thinning and losing ice mass since the Earth observation era using satellites. ICESat-2, equipped with the photon-counting altimetric technology, provides an unprecedented elevation accuracy of 2-4 cm and extremely high spatio-temporal coverages for reducing uncertainties in mass balance estimation of the ice sheet. We have developed a multi-temporal elevation change estimation model (MECEM) that is especially tailored for processing the ICESat-2 data and estimating mass changes. Here, we present our assessment of surface elevation change across the GrIS and its peripheral glaciers, using ICESat-2 observations acquired between March 2019 and March 2024. A validation against GNSS-derived elevation change rates near the Summit Station during 2022–2024 demonstrates a close agreement. In addition, a comparison with independent elevation change products indicates a strong consistency, particularly over interior high-elevation regions. Our results reveal increased thinning in the southeast and southwest coastal regions and major outlet glacier systems, such as Jakobshavn Isbræ and Helheim Glacier. The ablation zone (< 1500 m) experiences a rapid thinning at an average rate of −0.48 ± 0.04 m yr⁻¹, while the interior region (≥ 1500 m) remains relatively stable with a slight thickening. The mean surface elevation change rate over the entire GrIS is −0.10 ± 0.02 m yr⁻¹. We further convert the surface elevation changes to ice mass changes by using corrections of firn air content and solid earth. A comparison with other studies and a discussion are also provided.

How to cite: Li, R., Liu, M., Chen, Q., He, Y., Wang, X., and Qiao, G.: Surface Elevation Changes and Mass Balance of the Greenland Ice Sheet from 2019 to 2024 from ICESat-2 Observations using a new MECEM model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8541, https://doi.org/10.5194/egusphere-egu26-8541, 2026.

EGU26-10038 | ECS | Posters on site | CR2.1

ISMIP7 SMBMIP: a preliminary comparison of Greenland ice sheet surface mass balance products 

Clara Lambin, Devon Dunmire, Naveen Senthil, Nicole Schlegel, Sophie Nowicki, and Brice Noël

Surface mass balance (SMB) of polar ice sheets is a key component in quantifying their contribution to global sea-level rise. Accurate, high-resolution projections of SMB are therefore required to force ISMIP7 ice sheet models. In this study, we present preliminary results from SMBMIP, a comparison of several high-resolution SMB products over the Greenland Ice Sheet within the ISMIP7 framework. These products include, among others, SMB projections from the regional climate model MAR, statistical downscaling of MAR and the Earth System Model CESM2, and machine-learning outputs. For a meaningful comparison, participating projections are based on a same CESM2 historical climate and emission scenario. The aim is to explore uncertainties, performance and efficiency of various modelling approaches.

How to cite: Lambin, C., Dunmire, D., Senthil, N., Schlegel, N., Nowicki, S., and Noël, B.: ISMIP7 SMBMIP: a preliminary comparison of Greenland ice sheet surface mass balance products, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10038, https://doi.org/10.5194/egusphere-egu26-10038, 2026.

EGU26-10199 | ECS | Orals | CR2.1

Comparison of GRACE/GFO- and RACMO-based seasonal mass anomalies over the coastal zone of Greenland 

Weiran Li, Pavel Ditmar, Michiel van den Broeke, Brice Noël, and Bert Wouters

Gravity Recovery and Climate Experiment (GRACE) and GRACE Follow-On (GFO) satellite missions, altogether referred to as GRACE hereafter, are a powerful tool to provide Greenland monthly mass anomaly estimates over a time span of more than two decades. Here we present a comparison between GRACE seasonal mass anomalies and surface mass balance (SMB) estimates from the Regional Atmospheric Climate Model RACMO2.3p2. The latter provides estimates of SMB and its individual components over Greenland with a daily temporal sampling and high spatial resolution, i.e. 5.5 km in the tundra area and 1 km over glaciated areas, using statistical downscaling. Our goals are to provide frameworks to independently evaluate the model and to estimate buffered water storage (BWS), i.e. temporal storage of meltwater in the deeper ice sheet system subject to discharge into the ocean during the melt season or soon thereafter.

The comparison spans the time interval between February 2003 and July 2022. Long-term (slow) trends are removed to exclude signals related to ice discharge variability and glacial isostatic adjustment (assuming the seasonal variability of these signals is negligible). The GRACE- and RACMO-based estimates are inverted into mean mass anomalies per calendar month to extract their typical seasonal patterns. The study area is limited to the coastal zone of Greenland, including the ice sheet ablation zone where signals related to BWS and under- or over-estimation of runoff are concentrated. The coastal zone is further divided into 12 areas for a detailed analysis. We compare the time series of seasonal patterns in terms of RMS differences, Pearson correlation coefficient, and Nash-Sutcliffe Efficiency (NSE). Over the entire coastal zone, the RMS difference is 13.7 Gt or 1.3 cm in terms of mean equivalent water height (about 14% of the total signal); the correlation coefficient and NSE are 0.992 and 0.980, respectively, indicating a sufficient match between the overall seasonal patterns of the two datasets. A few individual coastal zones also show a good agreement between GRACE- and RACMO-based estimates, with the RMS differences below 2 cm. In two northwestern coastal areas, however, GRACE- and RACMO-based mass anomalies show large discrepancies (e.g. NSE lower than 0.7), potentially due to an overestimation of modelled runoff. In two southwestern coastal areas, a mismatch is observed as well, with maximum differences occurring in July, in concert with the timing of BWS documented in earlier studies.

While previous studies already attempted to quantify BWS in Greenland, they did not account for the scaling of modelled runoff, introducing a biased estimation of BWS. In light of our study, a more comprehensive approach can be adopted for BWS quantification. Such an approach can also benefit from using other regional climate models for BWS estimation.

How to cite: Li, W., Ditmar, P., van den Broeke, M., Noël, B., and Wouters, B.: Comparison of GRACE/GFO- and RACMO-based seasonal mass anomalies over the coastal zone of Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10199, https://doi.org/10.5194/egusphere-egu26-10199, 2026.

EGU26-11304 | Posters on site | CR2.1

A Study on Summer Surface Temperature of Antarctic Ice Shelves Based on FY-3 Satellite: A Case Study of the Getz and Amery Ice Shelves 

Tingting Liu, Xiaohong Zhang, Xiaoping Pang, and Yuande Yang

The Getz Ice Shelf is a region of high surface melt potential, yet its annual melt days are typically fewer than 10. In contrast, the upstream region of the Amery Ice Shelf, which has similar latitude and altitude, is more prone to surface melting, with some areas recording over 50 melt days throughout the year. Ice surface temperature (IST) is a critical indicator of its surface energy budget and mass balance. To investigate the differences in IST between the Getz and Amery ice shelves, this study employed high-resolution thermal infrared data from the FY-3A MERSI-Ⅰ and FY-3D MERSI-Ⅱ satellites to retrieve summer IST over both ice shelves for 2008–2014 and 2019–2024, and conducted a comparative analysis of their spatiotemporal variation patterns. Time series analysis of the Getz Ice Shelf revealed no statistically significant IST trend in either period. However, an anomalous warming event exceeding 5 K was observed in March 2013, abruptly reversing the typical seasonal cooling and resulting in a higher monthly average IST for March than for February. Meteorological analysis linked this anomaly to an anticyclone in the Amundsen Sea, which drove strong poleward transport of moisture and heat. The consequent increase in mid- and low-level cloud cover enhanced downward longwave radiation, leading to rapid surface warming. Also for the Amery Ice Shelf, time series analysis revealed no statistically significant IST trend in either period. Comparative analysis of summer IST reveals similar average values for the Getz and Amery ice shelves, with Getz even warmer by nearly 2 K in some years. However, surface melting on Getz remains lower. Analysis incorporating precipitation data indicates that the Getz Ice Shelf receives significantly higher precipitation than the Amery Ice Shelf. The greater snowfall replenishes surface fresh snow, increases albedo, and thereby suppresses melting. This suggests that wet ice shelves surface with high accumulation have a higher temperature threshold for surface melting. Notably, surface precipitation over the Getz Ice Shelf during the summer warming period (October–December) showed a significant declining trend from 2012 to 2023. Given the absence of pronounced changes in IST, this reduction in precipitation may elevate the future risk of surface melting on the Getz Ice Shelf.

How to cite: Liu, T., Zhang, X., Pang, X., and Yang, Y.: A Study on Summer Surface Temperature of Antarctic Ice Shelves Based on FY-3 Satellite: A Case Study of the Getz and Amery Ice Shelves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11304, https://doi.org/10.5194/egusphere-egu26-11304, 2026.

EGU26-11424 | Orals | CR2.1

A New View from Within: Borehole Pressure Sensors and the Measurement of Glacier Mass Balance 

Bradley Lipovsky, Ben Brand, Justin Burnett, Nicolas Michel-Hart, Benjamin Smith, and Dale Winebrenner

High-sensitivity borehole pressure sensors provide a novel means of monitoring the surface mass balance (SMB) of Earth’s great ice sheets. When properly coupled to the ice, these instruments are expected to detect millimeter-scale changes in ice thickness corresponding to variations in snow accumulation. The Boussinesq solution guarantees that a pressure sensor buried at a depth of 1000 m will represent a spatially weighted average of surface mass load variations with an approximate radius of 1000 m at the surface. The sensing system itself consists of a pressure sensor connected to a pressure coupling element such as a sack filled with antifreeze. Once freeze-in related transients have passed, the internal fluid pressure in the sack reflects the full overburden stress exerted by the overlying ice column. Long term drift of the sensors requires special engineering attention and may be corrected for using some combination of pre-deployment pressurization, in situ calibration, and/or the use of multiple in situ sensors. We discuss deployment considerations using the IceDiver thermal melt probe for a potential deployment at Greenland Summit Station. The borehole SMB observatory described here supports altimetry-based inference of glacier mass change, provides a critical dataset for validating firn densification models, and establishes a fundamentally new approach to measuring glacier mass balance.

How to cite: Lipovsky, B., Brand, B., Burnett, J., Michel-Hart, N., Smith, B., and Winebrenner, D.: A New View from Within: Borehole Pressure Sensors and the Measurement of Glacier Mass Balance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11424, https://doi.org/10.5194/egusphere-egu26-11424, 2026.

EGU26-11626 | ECS | Orals | CR2.1

Evaluation of MARv3.14 over Greenland and the Impact of Model Resolution 

Guillaume Timmermans, Noël Brice, Christoph Kittel, Dethinne Thomas, Ghilain Nicolas, Lambin Clara, and Fettweis Xavier

Accurate simulation of the Greenland Ice Sheet (GrIS) surface mass balance (SMB) is essential for quantifying its contribution to sea-level rise. The regional atmospheric climate model MAR is widely used to study GrIS SMB changes and force ice-sheet models, highlighting the importance of assessing its performance and sensitivity to horizontal resolution. Here, we evaluate the latest MARv3.14 version at 5 km resolution and assess the impact of coarser resolutions (10–30 km) on simulated GrIS SMB and its components.

MAR outputs are evaluated against a range of independent observations, including in situ SMB measurements, automatic weather station records of near-surface meteorological variables, and satellite-derived melt extent and albedo products. At 5 km resolution, MAR reproduces observed SMB with a root-mean-square error of 0.53 m w.e. yr⁻¹. For near-surface meteorological variables and surface energy budget fluxes, model errors are smaller than the corresponding observed variability. The assimilation of bare-ice albedo, implemented in the latest MAR version, improves model performance in the ablation zone. Remaining biases in the accumulation zone suggest that improvements to the snow albedo scheme are further required. Simulated melt timing is consistent with satellite-based melt extent products.

Comparing simulations at different spatial resolutions, we find that SMB discrepancies mainly occur at the ice-sheet margins, characterized by strong topographic gradients. While integrated SMB differences generally remain within interannual variability, precipitation and runoff are highly sensitive to the model spatial resolution.

Corrections based on a vertical SMB gradient (as in Franco et al., 2012) or a sub-pixel methodology allowing the surface scheme (SISVAT) to be run at a higher resolution than the atmospheric model could deal in part with runoff discrepancies vs spatial resolution but precipitation anomalies remain a challenge. We conclude by discussing ongoing model developments, in particular the implementation of a sub-pixel methodology.

 

How to cite: Timmermans, G., Brice, N., Kittel, C., Thomas, D., Nicolas, G., Clara, L., and Xavier, F.: Evaluation of MARv3.14 over Greenland and the Impact of Model Resolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11626, https://doi.org/10.5194/egusphere-egu26-11626, 2026.

EGU26-12210 | ECS | Posters on site | CR2.1

Updated Climatology and Surface Mass Balance for the period 1979-2024 of the Antarctic Peninsula using RACMO2.4p1 

Koen van der Aa, Carleen Reijmer, Peter Kuipers Munneke, Willem Jan van de Berg, and Christiaan van Dalum
In this contribution, we present a novel simulation with RACMO2.4p1 of the present-day Antarctic Peninsula (AP) climate, including the surface energy balance (SEB) and surface mass balance (SMB) of glacier and ice shelf surfaces. These model results can be used for estimating freshwater fluxes into the ocean, integrated glacier SMB, and regional climate patterns and trends, for the period 1979-2024 at a 5.5 km grid resolution.
The AP is the warmest region of Antarctica and has been subject to major calving events, notably in 1995 and 2002 (breakup of Larsen A and B, respectively), and in 2017 (breakoff of the A68 iceberg from Larsen C). Mass loss from the Eastern AP is mainly driven by atmospheric warming, as opposed to oceanic warming in the Western AP. Accurate estimates of the SEB and SMB are therefore essential to study the future stability of Eastern AP ice shelves. Our main objective is to explain the simulated and observed melt patterns over Larsen C. To that end, we investigate the temporal trends and spatial variability in SMB components over the simulated period, evaluated with the AntSMB dataset. We connect this to the SEB components, which we evaluate using automatic weather station (AWS) data starting in 2009.
We find good agreement with temperature (bias = -1.1 K, RMSE = 3.6 K) and wind speed (bias = +0.1 m s-1, RMSE = 2.6 m s-1) observations from the AntAWS dataset, as well as with the observed melt energy on Larsen C at the IMAU AWS stations (bias = +0.2 W m-2, RMSE = 6.8 W m-2). However, substantial biases remain in terms of downward longwave radiation and sensible heat flux (-18.7 W m-2 and +8.7 W m-2, respectively). Furthermore, we find large variability in mean annual temperature (SD = 1.3 K), SMB (SD = 61.0 mm w.e. yr-1), and melt (SD = 100.5 mm w.e. yr-1) on Larsen C. As a result, the data provide no evidence of statistically significant temporal trends for these variables over the period 1979-2024, which is consistent with earlier reports on natural variability on the AP. Our updated monthly SEB and SMB fields will become publicly available and will form the basis for future studies on the evolution of the Larsen C firn layer.

How to cite: van der Aa, K., Reijmer, C., Kuipers Munneke, P., van de Berg, W. J., and van Dalum, C.: Updated Climatology and Surface Mass Balance for the period 1979-2024 of the Antarctic Peninsula using RACMO2.4p1, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12210, https://doi.org/10.5194/egusphere-egu26-12210, 2026.

EGU26-12329 | ECS | Orals | CR2.1

Control of snow albedo decay on Greenland surface melt using the land surface model ORCHIDEE 

Philippe Conesa, Cécile Agosta, Sylvie Charbit, and Simon Beylat

The Greenland ice sheet (GrIS) constitutes a major contributor to sea level rise, with significant mass losses dominated by surface melt and runoff over recent decades. The enhanced surface melt is concomitant with an observed decrease in albedo and a retreat of the snow line to higher elevations, amplified by melt-albedo feedbacks. A realistic representation of snow and ice albedo over the GrIS is therefore essential in climate models to correctly represent the surface energy balance, the meltwater production and the ice sheet surface mass balance.

In ORCHIDEE, the land surface component of the IPSL-CM Global Climate Model, snow albedo is currently represented with a decay parameterization based on snow age. Such simplified parametrizations are common in land surface schemes of CMIP earth system models. Our objective is to improve the representation of snow albedo over the GrIS using observations from PROMICE stations and MODIS retrievals. Our approach relies on the use of the History Matching calibration tool, based on Gaussian processes emulators, to identify the snow albedo parameters best adapted to Greenland conditions.

We first perform an offline calibration over Greenland to assess the ability of the ORCHIDEE model to reproduce the snow albedo decay  and the bare ice extent in summer. We show that a single year calibration allows for a good representation of snow albedo decay over the 2000–2019 period. We aim to revisit this approach by using the atmospheric component of IPSL-CM, LMDZ, coupled with ORCHIDEE, in a regional configuration. This will allow us to assess whether atmosphere-surface feedback needs to be taken into account during the calibration procedure. Finally, we assess if the improved representation of albedo decay enables the IPSL model to produce a more realistic decrease of the GrIS surface mass balance over recent decades.

How to cite: Conesa, P., Agosta, C., Charbit, S., and Beylat, S.: Control of snow albedo decay on Greenland surface melt using the land surface model ORCHIDEE, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12329, https://doi.org/10.5194/egusphere-egu26-12329, 2026.

EGU26-13516 | ECS | Posters on site | CR2.1

Changes in Greenland firn densification from extended IMAU-FDM runs (1939-2023) 

Elizabeth Case, Peter Kuipers-Munneke, Max Brils, Willem-Jan van de Berg, Carleen Tijm-Reijmer, and Michiel van den Broeke

Firn densification turns snow into glacial ice. At the surface of ice sheets, ice caps, and glaciers, firn modulates the interaction between atmosphere and ice, and is in turn affected by temperature, precipitation, wind, deposition, and ice dynamics. As climatic factors vary, the rate of firn densification changes even as the mass stays constant. These densification rates are used to correct satellite altimetry measurements of mass balance across the Greenland and Antarctic Ice Sheets. The IMAU Firn Densification Model (IMAU-FDM) is a 1D, semi-empirical model that simulates the evolution of snow grain size, firn density, firn air content, temperature, and liquid water content commonly used for continent-wide altimetry corrections. We will present the results of the FDM from an extended timeseries (1939-2023) and updated forcing (ERA5-forced RACMO2p3.2), along with a toolkit for post-processing and using the output. We show the impact of longer-term forcing changes the overall firn air content and densification rates, and the effects of a longer, earlier spinup period. 

How to cite: Case, E., Kuipers-Munneke, P., Brils, M., van de Berg, W.-J., Tijm-Reijmer, C., and van den Broeke, M.: Changes in Greenland firn densification from extended IMAU-FDM runs (1939-2023), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13516, https://doi.org/10.5194/egusphere-egu26-13516, 2026.

EGU26-13635 | ECS | Posters on site | CR2.1

Spatio-temporal variability of surface energy and mass balance at Rutor Glacier (Italian Alps) 

Matteo Bertagni, Flavia Marini, Stefania Tamea, and Carlo Camporeale

Understanding melt processes and their contribution to runoff in glacierized catchments requires accounting for the strong spatial variability of surface energy exchanges. In this study, we analyse the spatial distribution of surface energy and mass balance at Rutor Glacier, the sixth-largest glacier in the Italian Alps, using field observations and a spatially distributed, physically based modelling framework.

The model combines in situ meteorological measurements collected at different elevations with high-resolution topographic information derived from a 5 m digital elevation model. Surface energy and mass-balance components are solved across the glacier surface to investigate how elevation, slope, and aspect influence melt patterns. Simulations are conducted for two consecutive hydrological years (September 2023–August 2024 and September 2024–August 2025), allowing an assessment of interannual variability in surface energy exchanges and melt dynamics.

The analysis focuses on characterizing spatial patterns of surface energy balance and surface melting, exploring their implications for meltwater production at the cell and watershed scales. Modelled meltwater fluxes are compared with available discharge observations to evaluate the consistency between simulated melt dynamics and field-based hydrological signals. Results and their relevance for snow- and glacier-fed runoff generation in mountain catchments will be discussed.

How to cite: Bertagni, M., Marini, F., Tamea, S., and Camporeale, C.: Spatio-temporal variability of surface energy and mass balance at Rutor Glacier (Italian Alps), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13635, https://doi.org/10.5194/egusphere-egu26-13635, 2026.

EGU26-17009 | Posters on site | CR2.1

Surface Mass Balance Model CISSEMBEL linking ice sheets and ESMs: Results of standalone GrSMBMIP simulations 

Christian Rodehacke, Kristiina Verro, Nicolaj Hansen, Uta Krebs-Kanzow, and Ruth Mottram

When you want to know the future of the Greenland ice sheet, you are confronted with the question: What will be Greenland's surface mass balance (SMB) in the future? 

The Copenhagen Ice-Snow Surface Energy and Mass Balance Model (CISSEMBEL) is a unified surface mass balance model developed at the Danish Meteorological Institute (DMI) that serves dual purposes in climate modeling. First, it operates as a standalone model to compute surface mass balance (SMB) from a wide range of atmospheric forcing data, including reanalysis products, meteorological forecasts, and automatic weather station (AWS) observations. Second, it acts as an innovative coupling framework that integrates SMB modeling into an atmospheric model. Since CISSEMBEL corrects dynamically elevation differences between the coarsely resolved orography in global atmosphere models and the high-resolution target during runtime, CISSEMBEL delivers boundary conditions essential for accurate atmosphere-ice sheet interactions. Ultimately, it enables a seamless integration of Ice Sheet Models (ISMs) into Earth System Models (ESMs).

In this presentation, we show CISSEMBEL results following the protocol of the Greenland Ice Sheet (GrIS) SMB model intercomparison project (GrSMBMIP). We present results on the grid of the used EraInterim (EraI) forcing as well as higher-resolution simulations on an Ice Sheet Model Intercomparison (ISMIP) grid. Our model results show that initialization affects the final results. Also, the different downscaling approaches (directly to a higher-resolution target or via height classes) available in CISSEMBEL deliver similar results. Since various parameterizations are available, the user can analyze their impact on results and explore the consequences on the SMB that determines Greenland’s future.

How to cite: Rodehacke, C., Verro, K., Hansen, N., Krebs-Kanzow, U., and Mottram, R.: Surface Mass Balance Model CISSEMBEL linking ice sheets and ESMs: Results of standalone GrSMBMIP simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17009, https://doi.org/10.5194/egusphere-egu26-17009, 2026.

EGU26-18429 | ECS | Orals | CR2.1

Emulating Surface Mass Balance in the Antarctic Peninsula Under Changing Forcings: A Transferability Assessment 

Emma Zirkel, Ruth Mottram, Kristiina Verro, and Stef Lhermitte

Regional climate models (RCM) with good snow schemes can provide high-resolution surface mass balance (SMB) estimates over Antarctica, but come with high computational costs limiting the number of realizations across Earth System Models (ESM) and shared socioeconomic pathways (SSP). SMB’s great local variability as observable in regions characterized by complex topography such as the Antarctic Peninsula, requires high resolution. Recent machine learning approaches have shown promising downscaling results as cost efficient alternative to RCMs. However, their limited transferability across forcings remains a drawback for practical application.

Here, we investigate transferability of a Convolutional Neural Network (CNN) based emulator predicting SMB over the Antarctic Peninsula utilizing multiple SSPs. Two training scenarios are compared: a) a perfect model setup where training and prediction are performed under the same SSP, and b) an imperfect model setup in which the emulator is trained on a higher emission scenario and applied to a lower emission scenario. The latter represents an interpolation along SSPs, therefore comparable performance to the perfect model setup is expected.

Preliminary analyses suggest consistency in large-scale statistics over the full domain with benchmarks set in earlier studies. However, pronounced local variability in model performance is observable, particularly in regions of high melt or precipitation. Ongoing work aims to quantify these differences, detect potential causes, and their implications for predictions in the imperfect model setup.

Positive results could enable the generation of additional SSP-runs from existing RCM simulations, therefore substantially reducing total computational cost relative to the number of predictions.

 

How to cite: Zirkel, E., Mottram, R., Verro, K., and Lhermitte, S.: Emulating Surface Mass Balance in the Antarctic Peninsula Under Changing Forcings: A Transferability Assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18429, https://doi.org/10.5194/egusphere-egu26-18429, 2026.

EGU26-21387 | ECS | Orals | CR2.1 | Highlight

A physics-guided Deep Learning Model for SMB of Central West Greenland 

Anna Puggaard, Anne Solgaard, Louise S. Sørensen, Ruth Mottram, and Sebastian B. Simonsen

Direct observations of the surface mass balance (SMB) over the Greenland Ice Sheet are currently limited to basin-scale estimates and sparse in situ measurements, making a comprehensive observational assessment challenging. Therefore, RCMs remain the best option for producing spatially and temporally continuous SMB estimates, but models show substantial regional differences, even under present-day conditions. While satellite observations provide extensive information about surface processes, a fully satellite-based SMB product remains to be seen.

In this study, we present SMBnet, a deep learning model that estimates SMB over central West Greenland by integrating satellite observations, reanalysis data, and simple physical constraints. SMBnet combines satellite-derived ice surface temperature and albedo with ERA5 reanalysis data, ice velocity, and GRACE/-FO mass anomalies to produce spatially and temporally continuous SMB estimates. The model employs a U-Net architecture and is trained using multiple loss terms that enforce consistency with observations and incorporate physical knowledge of accumulation and ablation processes. Although applied here to central West Greenland, the approach shows clear potential for extending it to the entire ice sheet, offering a computationally efficient, observation-driven complement to traditional RCMs for estimating present-day SMB.

How to cite: Puggaard, A., Solgaard, A., S. Sørensen, L., Mottram, R., and B. Simonsen, S.: A physics-guided Deep Learning Model for SMB of Central West Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21387, https://doi.org/10.5194/egusphere-egu26-21387, 2026.

EGU26-1720 | Orals | CR2.2

The Antarctic Peninsula under present day climate and future low, medium-high and very high emissions scenarios 

Bethan Davies and the Antarctic Peninsula under present day climate and future low, medium-high and very high emissions scenarios team

The Antarctic Peninsula is warming rapidly, with more frequent extreme temperature and precipitation events, reduced sea ice, glacier retreat, ice shelf collapse, and ecological shifts. Here, we review its behaviour under present-day climate, and low (SSP 1-2.6), medium-high (SSP 3-7.0) and very high (SSP 5-8.5) future emissions scenarios, corresponding to global temperature increases of 1.8°C, 3.6°C and 4.4°C by 2100. Higher emissions will bring more days above 0°C, increased liquid precipitation, ocean warming, and more intense extreme weather events such as ocean heat waves and atmospheric rivers. Surface melt on ice shelves will increase, depleting firn air content and promoting meltwater ponding. Under the highest emission scenario, collapse of the Larsen C and Wilkins ice shelves is likely by 2100 CE, and loss of sea ice and ice shelves around the Peninsula will exacerbate the current trends of land-ice mass loss. Collapse of George VI Ice Shelf by 2300 under SSP 5-8.5 would substantially increase sea level contributions. Under this very high emissions scenario, sea level contributions from the Peninsula could reach 7.5 ± 14.1 mm by 2100 CE and 116.3 ± 66.9 mm by 2300 CE. Conversely, under the lower emissions scenarios, the Antarctic Peninsula’s sea ice remains similar to present, and land ice is predicted to undergo only minor grounding line recession and thinning. Changes in sea surface temperatures and the change from snow to rain will impact marine and terrestrial biota, altering species richness and enhancing colonisation by non-native species. Ranges of key species such as krill and salps are likely to contract to the south, impacting their marine vertebrate predators. These changing conditions will also influence Antarctic Peninsula research, fisheries, tourism, infrastructure and logistics. The future of the Peninsula depends on the choices made today. Limiting temperatures to below 2°C, and as close as possible to 1.5°C (by following the SSP 1-1.9 or 1-2.6 scenarios), combined with effective governance, will result in increased resilience and relatively modest changes. Any higher emissions scenarios will damage pristine systems, cause sustained, irreversible ice loss on human timescales, and spread to Antarctic regions beyond the Peninsula.

How to cite: Davies, B. and the Antarctic Peninsula under present day climate and future low, medium-high and very high emissions scenarios team: The Antarctic Peninsula under present day climate and future low, medium-high and very high emissions scenarios, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1720, https://doi.org/10.5194/egusphere-egu26-1720, 2026.

EGU26-2576 | Posters on site | CR2.2

Extending the range and reach of physically-based Greenland ice sheet sea-level projections 

Heiko Goelzer, Constantijn J. Berends, Fredrik Boberg, Gael Durand, Tamsin L. Edwards, Xavier Fettweis, Fabien Gillet-Chaulet, Quentin Glaude, Philippe Huybrechts, Sébastien Le clec’h, Ruth Mottram, Brice Noël, Martin Olesen, Charlotte Rahlves, Jerem Rohmer, Michiel van den Broeke, and Roderik S. W. van de Wal

We present an ensemble of physically-based ice sheet model projections for the Greenland ice sheet (GrIS) that was produced as part of the European project PROTECT. Our ice sheet model (ISM) simulations are forced by high-resolution regional climate model (RCM) output and other climate model forcing, including a parameterisation for the retreat of marine-terminating outlet glaciers. The experimental design builds on the Ice Sheet Model Intercomparison Project for CMIP6 (ISMIP6) protocol and extends it to more fully account for uncertainties in sea-level projections. We include a wider range of CMIP6 climate model output, more climate change scenarios, several climate downscaling approaches, a wider range of sensitivity to ocean forcing and we extend projections beyond the year 2100 up to year 2300, including idealised overshoot scenarios. GrIS sea-level rise contributions range from 16–76 mm (SSP1-2.6/RCP2.6), 22–163 mm (SSP2-4.5) and 27–354 mm (SSP5-8.5/RCP8.5) in the year 2100 (relative to 2014). The projections are strongly dependent on the climate scenario, moderately sensitive to the choice of RCM, and relatively insensitive to the ice sheet model choice. In year 2300, contributions reach 49 to 3127 mm, indicative of large uncertainties and a potentially very large long-term response. Idealised overshoot experiments to 2300 produce sea-level contributions in a range from 49 to 201 mm, with the ice sheet seemingly stabilised in a third of the experiments. Repeating end of the 21st century forcing until 2300 results in contributions of 58–163 mm (repeated SSP1-2.6), 98–218 mm (repeated SSP2-4.5) and 282–1230 mm (repeated SSP5-8.5). The largest contributions of more than 3000 mm by year 2300 are found for extreme scenarios of extended SSP5-8.5 with unabated warming throughout the 22nd and 23rd century. We also extend the ISMIP6 forcing approach backwards over the historical period and successfully produce consistent simulations in both past and future for three of the four ISMs. The ensemble design of ISM experiments is geared towards the subsequent use of emulators to facilitate statistical interpretation of the results and produce probabilistic projections of the GrIS contribution to future sea-level rise.

How to cite: Goelzer, H., Berends, C. J., Boberg, F., Durand, G., Edwards, T. L., Fettweis, X., Gillet-Chaulet, F., Glaude, Q., Huybrechts, P., Le clec’h, S., Mottram, R., Noël, B., Olesen, M., Rahlves, C., Rohmer, J., van den Broeke, M., and van de Wal, R. S. W.: Extending the range and reach of physically-based Greenland ice sheet sea-level projections, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2576, https://doi.org/10.5194/egusphere-egu26-2576, 2026.

EGU26-3349 | ECS | Posters on site | CR2.2

The thermal memory of the Antarctic Ice Sheet 

Olivia Raspoet, Violaine Coulon, and Frank Pattyn

The Antarctic Ice Sheet has undergone significant climate variability throughout glacial-interglacial cycles. Because thermal diffusion and advection rates are low, surface temperature anomalies propagate slowly to the base, imparting a thermal memory to ice sheets that persists for thousands of years. Since ice temperature controls viscosity, deformation rates, and subglacial processes, this inherited thermal structure exerts a direct influence on contemporary ice dynamics. Recent work on the thermal state of the Antarctic Ice Sheet (Raspoet & Pattyn, 2025) has explored uncertainties in boundary conditions and model approximations, but considered a thermal steady state, thereby assuming equilibrium with present-day climatic conditions and neglecting the legacy of past glacial-interglacial changes. In this study, we employ the thermomechanical ice-sheet model Kori-ULB, driven by reconstructed transient climate forcings spanning the last interglacial to the present day, to quantify the effects of paleoclimatic evolution on the thermal state of the Antarctic Ice Sheet and assess the implications for ice-sheet dynamics and model initialization. Results show that englacial temperatures are sensitive to the past climate history, leading to uncertainties of the same order as those related to the geothermal heat flow. Incorporating variations in surface temperatures and accumulation rates over the last glacial-interglacial cycle results in colder temperature profiles and basal thermal conditions, suggesting that steady-state ice-sheet models may overestimate present-day thermal conditions.

References:

Raspoet O., Pattyn F. (2025), Estimates of basal and englacial thermal conditions of the Antarctic ice sheet. Journal of Glaciology 71, e104, 1–16. doi: 10.1017/jog.2025.10087

How to cite: Raspoet, O., Coulon, V., and Pattyn, F.: The thermal memory of the Antarctic Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3349, https://doi.org/10.5194/egusphere-egu26-3349, 2026.

EGU26-4033 | ECS | Orals | CR2.2

Simulation of the Greenland ice-sheet deglaciation constrained by past and present observables 

Lucía Gutiérrez-González, Ilaria Tabone, Jorge Alvarez-Solas, Marisa Montoya, Jan Swierczek-Jereczek, Sergio Pérez-Montero, Santiago Tesouro, Javier Blasco, and Alexander Robinson

The Greenland Ice Sheet (GrIS) has experienced accelerated mass loss in recent decades and is expected to become a major contributor to global sea-level rise over the coming century. Understanding its response to climate forcing in a global warming context has become critical, particularly for the adaptation of coastal communities worldwide.

The last deglaciation of the GrIS offers valuable insights into ice-climate interactions, as extensive paleoclimatic records document its retreat through a period of major climate changes. During this interval, the GrIS retreated from its extensive Last Glacial Maximum (LGM) configuration to its present state, passing through the Holocene Thermal Maximum (HTM) when temperatures exceeded present-day values and may have overshot the GrIS tipping point. Despite the large amount of paleoclimatic data available, ice-sheet models struggle in reproducing key aspects of the observational record, and the magnitude of the GrIS contribution to sea level during the HTM remains highly uncertain.

In this study, we evaluate an ensemble of 3000 ice-sheet simulations performed with the  ice-sheet model Yelmo against different observational constraints. These include: (1) LGM ice-sheet extent, (2) ice-core-derived surface elevations, (3) relative sea-level records, (4) retreat chronology based on the PaleoGrIS dataset, and (5) the present-day ice-sheet configuration (ice thickness, ice velocity, and bedrock uplift rates). By identifying the simulations that best match these constraints, we provide a geologically-constrained reconstruction of the GrIS during the last deglaciation.

How to cite: Gutiérrez-González, L., Tabone, I., Alvarez-Solas, J., Montoya, M., Swierczek-Jereczek, J., Pérez-Montero, S., Tesouro, S., Blasco, J., and Robinson, A.: Simulation of the Greenland ice-sheet deglaciation constrained by past and present observables, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4033, https://doi.org/10.5194/egusphere-egu26-4033, 2026.

EGU26-5356 | Orals | CR2.2

Stability of the Greenland and Antarctic ice sheets when dynamically coupled through the Atlantic meridional overturning circulation. 

Sergio Pérez-Montero, Jorge Alvarez-Solas, Alexander Robinson, and Marisa Montoya

Climate change challenges all Earth subsystems. The Greenland and Antarctic ice sheets together with the Atlantic Meridional Overturning Circulation are subsystems of particular concern, as they are subject to tipping points, i.e., thresholds above which their current state changes to another that is qualitatively and quantitatively different. Their stability has been studied in depth through offline (stand-alone) modeling and “one-way” coupling with each other. However, we know that in the past, the Northern and Southern hemispheres have interacted through the bipolar seesaw. Thus, these subsystems have the potential to interact with each other, but this relationship is challenging to simulate. Here we investigate the behavior of a simplified approach coupling the state-of-the-art ice-sheet model Yelmo with an ocean box model and, importantly, vice versa. We will show the results of exposing the system to various climate change scenarios in order to see how different ice timescale responses alter the coupled stability. 

How to cite: Pérez-Montero, S., Alvarez-Solas, J., Robinson, A., and Montoya, M.: Stability of the Greenland and Antarctic ice sheets when dynamically coupled through the Atlantic meridional overturning circulation., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5356, https://doi.org/10.5194/egusphere-egu26-5356, 2026.

EGU26-5397 | Orals | CR2.2

Evaluation of albedo and elevation feedbacks on Greenland complete deglaciation in a CMIP model: comparison of coupled and uncoupled simulations  

Miren Vizcaino, Michele Petrini, Raymond Sellevold, Thirza Feenstra, Bert Wouters, Katherine Thayer-Calder, William Lipscomb, and Gunter Leguy

We present here a multi-century simulation of future Greenland ice sheet evolution under 4xCO2 forcing with the Community Earth System Model version 2 bi-directionally coupled to the Community Earth Sheet Model version 2 (CESM2-CISM2). We examine the evolution of global climate, ice sheet topography and flow, as well as the individual components of the surface mass and energy balance. We compare results with a simulation with uni-directional coupling, where the atmosphere and land components see a prescribed pre-industrial ice sheet topography, and the ocean sees prescribed pre-industrial freshwater fluxes corresponding to the initial CESM2-CISM2 state in the two-way coupled baseline simulation. We find that albedo feedback causes the solar flux to be the primary energy contributor to total melt of the ice sheet. Changes in ice sheet elevation reduce the input of snowfall to the ice sheet due to enhanced rain over snow partition of precipitation. Changes in elevation cause more than doubling of melt rates after the ice sheet area has decreased by more than 50%.

How to cite: Vizcaino, M., Petrini, M., Sellevold, R., Feenstra, T., Wouters, B., Thayer-Calder, K., Lipscomb, W., and Leguy, G.: Evaluation of albedo and elevation feedbacks on Greenland complete deglaciation in a CMIP model: comparison of coupled and uncoupled simulations , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5397, https://doi.org/10.5194/egusphere-egu26-5397, 2026.

EGU26-5653 | Posters on site | CR2.2

FirnMelt: Greenland’s Melting Firn and Ice Sheet Response 

Horst Machguth and the The FirnMelt Team

Firn currently covers almost 90 % of the surface of the Greenland Ice Sheet. Most of Greenland’s firn plateau experienced only occasional melt in the past but ever rising temperatures increase melting and it is uncertain how a future melting firn plateau will impact ice sheet mass balance, hydrology and ice dynamics. Assessing these impacts requires coupling firn models to ice sheet hydrology and ice dynamics models.

The FirnMelt ERC Synergy project will assess the Greenland Ice Sheet’s reaction to increased melting across its vast firn plateau. The project starts in April 2026 and will last for six years. The project is led by four PIs and will involve about 20 scientific and technical staff. Here we detail planned methods, models and timeline of the five overarching project tasks, namely (i) large-scale in situ and remote sensing measurements of all types of firn and meltwater discharge, (ii) parameterizing melting firn based on these measurements, (iii) develop firn models able to simulate melting firn and firn meltwater discharge in three dimensions, (iv) embedding these models into a ice-sheet model suite where they are coupled to ice sheet hydrology and ice dynamics, and (v) calculating how Greenland’s melting firn plateau will impact the entire ice sheet and its sea level contribution, until the year 2300.

How to cite: Machguth, H. and the The FirnMelt Team: FirnMelt: Greenland’s Melting Firn and Ice Sheet Response, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5653, https://doi.org/10.5194/egusphere-egu26-5653, 2026.

EGU26-7003 | ECS | Posters on site | CR2.2

ADMIRE: Improving Antarctic mass balance projections by coupling a Deep Learning basal melt emulator with the Kori-ULB ice sheet model 

Christoph Kittel, Clara Burgard, and Violaine Coulon

The future contribution of the Antarctic Ice Sheet to global sea-level rise remains the largest source of uncertainty in climate projections. This uncertainty is primarily driven by the complex interaction between the ocean and the ice shelf cavities. Most ice sheet models still rely on simplified melt parameterizations that fail to capture the complex oceanographic processes within sub-ice-shelf cavities, while fully coupled ice-ocean models remain too computationally expensive for large-scale sensitivity studies. In this study, we present ADMIRE (Antarctic Deep MELT and Ice REpresentation), a new ongoing-work intermediate-complexity framework. ADMIRE couples the ice sheet model Kori-ULB with DeepMELT, a deep learning emulator trained on high-resolution NEMO-SI3 simulations. This coupling allows for a more physically consistent representation of the ice-ocean interface at a fraction of the computational cost of a coupled ice-sheet-ocean model. We compare the sensitivity of the Antarctic grounding line migration and overall mass balance when using the DeepMELT emulator versus traditional melt parameterizations. Furthermore, we investigate the impact of temporal coupling steps and interpolation methods on the projections. Our preliminary results highlight the potential of machine learning-based emulators to bridge the gap between simple parameterizations and complex coupled models, providing more robust projections of Antarctica’s future but at a low computational cost, allowing for comprehensive and multi-century studies.

How to cite: Kittel, C., Burgard, C., and Coulon, V.: ADMIRE: Improving Antarctic mass balance projections by coupling a Deep Learning basal melt emulator with the Kori-ULB ice sheet model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7003, https://doi.org/10.5194/egusphere-egu26-7003, 2026.

EGU26-7109 | ECS | Orals | CR2.2

Coupled Climate-Ice-Sheet Simulations Reveal Novel Teleconnection Between Northern Hemisphere Ice Sheets and the Antarctic Ice Sheet 

Pierre Testorf, Clemens Schannwell, Marie-Luise Kapsch, and Uwe Mikolajewicz

Coupled climate-ice-sheet modeling is still in its developing stage, and feedback processes between ice sheets and climate are still not yet fully understood. Here, we use simulations with a coupled climate-ice-sheet model to investigate teleconnections between Northern Hemispheric ice sheets and the Antarctic ice sheet (AIS) without direct freshwater forcing. We show that ice mass removal in the Northern Hemisphere can alter AIS evolution through a series of feedbacks. Changes in surface properties and orographic effects warm the newly deglaciated areas and the North Atlantic Ocean at mid-depth. The warmer water masses propagate to the Southern Ocean, where internal oscillations periodically deliver them to the Antarctic coast. These repeated warm water intrusions destabilize the Ross ice shelf, ultimately triggering a runaway retreat of the West Antarctic ice sheet. Our results underscore the importance of coupled bi-hemispheric climate-ice-sheet modeling to capture global teleconnections between ice sheets and climate.

How to cite: Testorf, P., Schannwell, C., Kapsch, M.-L., and Mikolajewicz, U.: Coupled Climate-Ice-Sheet Simulations Reveal Novel Teleconnection Between Northern Hemisphere Ice Sheets and the Antarctic Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7109, https://doi.org/10.5194/egusphere-egu26-7109, 2026.

EGU26-7112 | ECS | Posters on site | CR2.2

Exploring ice-atmosphere feedbacks in Antarctica using coupled simulations 

Violaine Coulon and Christoph Kittel
  • 2Laboratory of climatology, SPHERES research unit, Department of Geography, University of Liège, Liège, Belgium
  • 3Physical Geography Research Group, Department of Geography, Vrije Universiteit Brussel, Brussels, Belgium

Accurate projections of the Antarctic ice sheet contribution to future sea-level rise require a robust representation of ice–atmosphere interactions and associated surface mass balance (SMB) feedbacks. Although they remain computationally expensive, coupled ice–atmosphere simulations provide the ideal framework for capturing these processes.
In this work in progress, we present ongoing coupled simulations between the ice-sheet model Kori-ULB and the regional climate model MAR. The coupled Kori-MAR simulations are conducted over Antarctica for the period 1980–2100 and are forced by the IPSL-CM6A-LR climate model under the SSP5-8.5 scenario. We compare the coupled simulations with three simplified modelling approaches: (i) ice-sheet model experiments externally forced by MAR outputs assuming a fixed ice-sheet geometry, (ii) simulations using a positive degree-day (PDD) scheme forced directly by IPSL-CM6A-LR, and (iii) simulations using a PDD scheme forced by MAR(IPSL-CM6A-LR). This allows us to investigate the influence of ice geometry changes on Antarctic SMB and projected ice-sheet mass loss. In parallel, we assess the ability of simplified SMB methods to reproduce MAR-derived SMB fields and their temporal evolution. A key objective is to better constrain the melt–elevation feedback emerging in the coupled simulations and to use this information to calibrate and improve PDD-based approaches for long-term Antarctic ice-sheet projections.

How to cite: Coulon, V. and Kittel, C.: Exploring ice-atmosphere feedbacks in Antarctica using coupled simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7112, https://doi.org/10.5194/egusphere-egu26-7112, 2026.

EGU26-7333 | ECS | Orals | CR2.2

The contribution of the Antarctic Ice Sheet to global sea level from the Last Glacial Cycle to the future 

Santiago Tesouro, Jorge Álvarez-Solas, Javier Blasco, Alexander Robinson, Jan Swierczek-Jereczek, and Marisa Montoya

The Antarctic Ice Sheet (AIS) is the largest potential contributor to future sea-level rise, with an ice volume equivalent to 58 m of global-mean sea level. However, high uncertainties arise from the representation of key physical processes in ice-sheet models, such as basal sliding, ice-ocean interactions, and feedback mechanisms associated with glacial isostatic adjustment (GIA). Previous studies have estimated the future Antarctic sea-level contribution (SLC) by forcing an ice sheet spun up to a present-day equilibrium state. However, observations of the last decades indicate that the AIS is not in equilibrium, as it is undergoing net mass loss as a result of both ongoing anthropogenic climate change and its long-term adjustment following the last deglaciation. Here, we study the future SLC of the AIS using simulations that span a complete Last Glacial Cycle. To this end, we use the ice-sheet model Yelmo coupled to the GIA model Fastisostasy, and construct an ensemble that accounts for uncertainties in process representation. The model is forced using the PMIP3 ensemble-mean reconstruction of the Last Glacial Maximum (LGM) and the present-day climate, weighted by an index derived from Antarctic ice-core records. The simulations are initiated in the Last Interglacial and evaluated based on their consistency with geological constraints from the LGM and the deglaciation, as well as present-day observations of the AIS. Using these paleo-constrained model configurations, we then investigate the response of the AIS to different future climate-change scenarios.

How to cite: Tesouro, S., Álvarez-Solas, J., Blasco, J., Robinson, A., Swierczek-Jereczek, J., and Montoya, M.: The contribution of the Antarctic Ice Sheet to global sea level from the Last Glacial Cycle to the future, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7333, https://doi.org/10.5194/egusphere-egu26-7333, 2026.

EGU26-7719 | ECS | Orals | CR2.2

Impacts of freshwater fluxes on ice shelves tipping points in UKESM  

Thi Khanh Dieu Hoang, Robin S. Smith, Kaitlin A. Naughten, and Colin G. Jones

There is a strong concern about how fast and how much the global sea level will rise in the next few decades due to the current global warming. However, the projection range is large due to uncertainties about the future evolution of the Antarctic ice sheet, particularly the possibility of the ice shelves' collapse.  

With the base submerged in seawater, these ice shelves are strongly influenced by the surrounding oceanic conditions, which can be split into two regimes: cold or warm cavity. When ice shelves are exposed to warm water, basal melt increases sharply, leading to a loss of buttressing of the grounded ice upstream and potentially the collapse of the shelf. Results from TIPMIP (Tipping Points Modelling Intercomparison Project) idealised experiments carried out by the UK Earth System Model (UKESM) with an interactive Antarctic ice sheet component suggest that tipping points for several ice shelves will be reached in the future at relatively high global warming levels (GWLs). However, it is questionable whether the warming thresholds for tipping that we find are realistic due to the model biases and other uncertainties. 

This study focuses on exploring the uncertainty in the climate simulated by UKESM and assessing the consequences of ice shelf tipping on the wider Earth System. To do this, we induce the cavity regime shift at a lower GWL than the reported threshold by mimicking the key climate change forcing identified from the higher GWL experiments via an artificial freshwater around the Antarctic ice sheet margin. By doing so, we obtain a pair of low GWL experiments with and without ice shelf tipping, which allows us to isolate the impact of ice shelf tipping on the Earth System. In addition, the experiment setup also allows us to explore the consequences of different scenarios of various freshwater hosing values. The preliminary results indicate that the excessive freshwater induces an expansion of Southern Ocean sea ice, leading to a cooling trend in global mean temperature. 

How to cite: Hoang, T. K. D., Smith, R. S., Naughten, K. A., and Jones, C. G.: Impacts of freshwater fluxes on ice shelves tipping points in UKESM , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7719, https://doi.org/10.5194/egusphere-egu26-7719, 2026.

In order to predict future changes in the Antarctic Ice Sheet under anthropogenic climate change, it is essential that we understand how it
responded to past climatic changes. The Antarctic Peninsula is seen as a bellwether system for the wider Antarctic Ice Sheet and, as such, is an
ideal palaeo-glaciological study area. The timings of the retreat of the ice front in this area since the Last Glacial Maximum have been
extensively researched and the configuration of the major ice streams that drained the ice sheet on the Northern Peninsula is broadly known.
However, the ice-ocean interactions that occurred during this period remain poorly understood. The identification and analysis of iceberg
ploughmarks can provide information on the extent of past ice sheets and the morphology of their calving fronts; past calving regimes and
hence the dynamic behaviour of the ice sheet in the past and how this may have changed over time; and past ocean circulation. During a
Schmidt Ocean Institute scientific cruise to the Antarctic Peninsula, high resolution, multibeam acoustic data was acquired in a poorly mapped
area of the Bellingshausen Sea near the Ronne Entrance. Thousands of iceberg ploughmarks were identified on bathymetric maps produced
from this data. These scours were mapped and their morphological characteristics were recorded. Morphometric analyses were undertaken,
including quantitative investigations of length, depth, width and sinuosity, and the intensity and distribution of scours were also investigated.
The implications of these results for the morphology and dynamics of the ice sheet and ice-ocean interactions since the Last Glacial Maximum
are then discussed. The insights gained from this study will be used to help validate and constrain ice sheet models where these ice-ocean
interactions are not currently well represented.

How to cite: Timbs, R. and Montelli, A.: Insight into ice-ocean interactions during the Last Deglaciation revealed by iceberg ploughmarks identified on the continental shelf of the West Antarctic Peninsula, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7838, https://doi.org/10.5194/egusphere-egu26-7838, 2026.

EGU26-8317 | Orals | CR2.2

Northern Hemisphere ice-sheet dynamics during the last two deglaciations: responses to gradual and abrupt climate changes 

Lauren Gregoire, Violet Patterson, Brooke Snoll, Ruza Ivanovic, Niall Gandy, Yvan Rome, Frank Arthur, and Sam Sherriff-Tadano

The last two deglaciations mark transitions from glacial to interglacial climates, dramatically reshaping Northern Hemisphere ice sheets. Numerical modelling of these transitions provides critical insight into the processes controlling ice-sheet retreat and collapse. Comparing the last two deglaciations allows us to evaluate how different forcings and initial conditions influence ice-sheet dynamics and understand the interplay between orbital forcing, greenhouse gases, abrupt climate changes and ice sheet instabilities in driving ice sheet evolution.

We use the fast yet comprehensive coupled General Circulation Atmosphere–ice-sheet model FAMOUS–BISICLES to simulate the Northern Hemisphere ice-sheet evolution during the penultimate deglaciation (140–128 thousand years ago; ka) and the last deglaciation (21-7 ka), with particular interest in the abrupt Bølling warming (14.5 ka). Our simulations follow the PMIP4 (Palaeoclimate Model Intercomparison Project 4) protocols and are forced with prescribed sea surface temperatures and sea ice from transient climate model outputs to reduce biases and force millennial abrupt climate changes.

First, we compare the penultimate and last deglaciations to assess how orbital forcing, greenhouse gas concentrations, and uncertain model parameters and SST inputs shape both the pace and spatial patterns of ice retreat. Results indicate a faster ice retreat during the penultimate deglaciation. Sensitivity experiments show that the rate of deglaciation is particularly sensitive to processes that impact the surface mass balance, but ice dynamics also play an important role. Sub-shelf melt rate is less significant; however, it can be important where confined ice shelves are able to form. Although insolation drives the deglaciations, rising greenhouse gases and warming SSTs significantly amplify the ice-sheet response to orbital forcing.

Second, we focus on the abrupt Bølling warming (~14.5 ka). Our simulations show accelerated deglaciation during this event, though the magnitude of response depends on the ice-sheet topography during the warming and on the pattern of abrupt SST increase prescribed. Marine-based sections, particularly the Barents–Kara ice sheet, exhibit the greatest sensitivity to prescribed ocean changes.

How to cite: Gregoire, L., Patterson, V., Snoll, B., Ivanovic, R., Gandy, N., Rome, Y., Arthur, F., and Sherriff-Tadano, S.: Northern Hemisphere ice-sheet dynamics during the last two deglaciations: responses to gradual and abrupt climate changes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8317, https://doi.org/10.5194/egusphere-egu26-8317, 2026.

Mass loss from ice sheets under the ongoing anthropogenic warming is a major contributor to sea-level rise. Previous studies suggest that global warming exceeding 2 °C could push the marine-based West Antarctic Ice Sheet beyond a critical threshold, triggering irreversible retreat and multi-meter rise in the global-mean sea-level. Climate overshoot scenarios are a key focus of CMIP7, yet most existing work on the reversibility of ice sheets is based on quasi-equilibrium simulations, with much less attention paid to ice sheets' stability and reversibility under century-scale transient climate forcing. Here we use climate and ice sheet models to simulate the evolution of the Antarctic and Greenland ice sheets under multiple climate overshoot scenarios. Results show that net-negative emissions in overshoot pathways can substantially reduce ice loss from the Greenland Ice Sheet, but are less effective in mitigating retreat of the West Antarctic Ice Sheet. This indicates that the West Antarctic Ice Sheet may also exhibit a tipping behavior under overshoot scenarios, and that achieving carbon neutral early is crucial to avoiding a potential catastrophic sea-level rise.

How to cite: Li, D.: Stability and reversibility of ice sheets in climate overshoot scenarios, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8704, https://doi.org/10.5194/egusphere-egu26-8704, 2026.

EGU26-8750 | Posters on site | CR2.2

Developments and evaluation of ice sheet model IcIES2 for Antarctic configuration 

Takashi Obase, Fuyuki Saito, and Ayako Abe-Ouchi

We present our development of the Ice sheet model for Integrated Earth-system Studies (IcIES2) for the Antarctic ice sheet configuration as a model development for CMIP7-ISMIP7. The flow of the ice is calculated with the shallow ice approximation (SIA) and shallow shelf approximation (SSA). To represent the migration of grounding lines, we use the grounding line flux boundary condition of Schoof (2007), following previous implementations (Pollard and DeConto 2012; 2020). The ice velocity fields are calculated using a hybrid approach that combines the SIA and SSA approximations, based on the ratio of basal sliding velocity to the depth-averaged velocity from the SIA solution. We perform sensitivity experiments on ice-sheet model parameters using the present-day bedrock topography and surface mass balance to obtain a reasonable present-day Antarctic ice-sheet configuration. We also perform experiments with an abrupt increase in sub-shelf melting to evaluate the model response to reduced ice shelf buttressing and marine ice sheet instability.

How to cite: Obase, T., Saito, F., and Abe-Ouchi, A.: Developments and evaluation of ice sheet model IcIES2 for Antarctic configuration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8750, https://doi.org/10.5194/egusphere-egu26-8750, 2026.

EGU26-9160 | ECS | Posters on site | CR2.2

Surface melt outweighs ice discharge over the next three centuries in fully coupled MAR-GISM simulations 

Chloë Marie Paice, Xavier Fettweis, and Philippe Huybrechts

When studying the future evolution and sea level contribution of the Greenland ice sheet, a realistic representation of ice sheet–atmosphere interactions in simulations is crucial. Therefore, to analyse the ice sheet evolution over the coming three centuries, we have performed several fully coupled ice sheet–regional climate model simulations. Our two-way coupled MAR–GISM simulations were driven by IPSL-CM6A-LR output under the SSP5-8.5 scenario, available up to 2300, and outlet glacier retreat was included through an empirical retreat parametrization.

To disentangle the long-term importance of ice mass loss through surface mass balance (SMB) versus marine discharge, we compare simulations with only atmospheric or oceanic forcing to simulations with both forcings applied simultaneously. They indicate that both atmospheric and oceanic forcing individually still lead to a similar sea level contribution by 2100. But, by 2300 the SMB-driven ice mass loss is about five times larger than the discharge-driven ice mass loss in our simulations, as the ice sheet retreats on land and gradually loses contact with the ocean. Besides, an analysis of the SMB components and freshwater fluxes between simulations demonstrates that surface melting and ice discharge through the ice–ocean boundary are mutually competitive processes.

Lastly, in terms of total ice mass loss, the importance of the chosen sensitivity parameter in the retreat parametrization increases over time. Whereas the difference in ice mass loss contribution from SMB versus discharge attenuates between simulations of differing sensitivity, because surface melting becomes increasingly dominant relative to marine discharge. Nevertheless, our simulations indicate that the applicability of the empirical retreat parametrization, which was developed for recent observations, becomes questionable over time. 

How to cite: Paice, C. M., Fettweis, X., and Huybrechts, P.: Surface melt outweighs ice discharge over the next three centuries in fully coupled MAR-GISM simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9160, https://doi.org/10.5194/egusphere-egu26-9160, 2026.

EGU26-9804 | ECS | Posters on site | CR2.2

The impact of ice sheet thermal memory in Antarctica’s response to climate warming 

Martim Mas e Braga, Tijn Berends, Erwin Lambert, and Jorge Bernales

The magnitude of the Antarctic Ice Sheet's response to future climate scenarios in ice sheet models depends on the choice of initial and basal sliding conditions. Basal sliding cannot be directly measured but is instead commonly inferred from observed surface velocity or ice thickness assuming the ice sheet is in equilibrium with the modern climate. The inferred basal sliding field is also affected by assumptions of different model parameters and the ice rheology, which all impact the modelled ice sheet behaviour. Ice rheology is often treated as idealised, prescribed as uniform, or also inferred from velocity observations. Such approaches lead to either a non-unique problem or to compensating errors in the inferred fields due to intrinsic uncertainties in the observations.

To reduce compensating errors and not assume equilibrium with the modern climate, we force our ice sheet initial geometry with long-term temperature variations (i.e., a thermal spinup), thus generating a thermal structure (and therefore ice rheology) that is consistent with the ice sheet's long-term climate history. We assess different approaches to combine the thermal spinup with initialisation procedures for the Antarctic Ice Sheet, analysing their match to observed borehole temperatures at ice core sites. By initialising Antarctic Ice Sheet simulations with a thermal spinup, we improve our model’s initial conditions reducing the mismatch between modelled and observed ice sheet geometries and the uncertainty around the ice sheet's basal conditions and ice rheology with respect to basal and englacial temperatures. Finally, we use the different obtained initial states to show the impact of the ice sheet’s thermal history compared with idealised temperatures or equilibrium conditions on its sensitivity to future warming.

How to cite: Mas e Braga, M., Berends, T., Lambert, E., and Bernales, J.: The impact of ice sheet thermal memory in Antarctica’s response to climate warming, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9804, https://doi.org/10.5194/egusphere-egu26-9804, 2026.

The Mid-Pleistocene Transition (MPT) marks one of the most profound reorganizations of the Earth’s climate system over the Quaternary. During this interval, the dominant glacial-interglacial cyclicity shifted from 40 kyr to 100 kyr without a corresponding change in orbital forcing, implying fundamental internal feedbacks within the climate system. Post-MPT glaciations became longer (up to ~60 kyr), more severe, and characterized by larger and more stable Northern Hemisphere ice sheets. Despite intensive research into the mechanisms driving the MPT, the response of ocean trace metal cycling to Northern Hemisphere ice-sheet dynamics remains poorly constrained, limiting our ability to fully integrate ice-sheet evolution with changes in ocean circulation, elemental cycling, and the carbon cycle.

Here we present a new authigenic neodymium isotope (εNd) record from ODP Site 982 (1134 m water depth), spanning 1.4–0.6 Ma and capturing the MPT. Our record reveals clear and systematic glacial-interglacial εNd variability linked to the evolving Icelandic Ice Sheet (IIS) and its modulation of volcanic erosion and weathering fluxes into the NE Atlantic, coupled with southward shifts in deep-water formation during glacials. Before the MPT, interglacial εNd values of -13.5 to -12.5 indicate persistent influence of Labrador Sea-derived waters, whereas glacial intervals are marked by more radiogenic εNd from -11 around 1.4 Ma to -9 by 1.1 Ma, reflecting increasing Icelandic volcanic input influence associated with IIS expansion. From ~1.1 Ma onward, the εNd contrast between climate states intensifies and reaches its strongest amplitude, with interglacials becoming slightly more unradiogenic (to -14) and glacials reaching radiogenic values up to -8. This persistent pattern of radiogenic in glacials and unradiogenic in interglacials continues into later cycles, indicating that Icelandic volcanic weathering and IIS extent reached their maximum expression since the MPT. Our results demonstrate that the IIS exerted first-order control on NE Atlantic seawater Nd isotope cycling during glacial periods, and that this modulation strengthened across and after the MPT. Importantly, the gradual amplification of Icelandic erosion signals suggests that Northern Hemisphere ice-sheet expansion (at least in Iceland) was a response to, rather than the initial trigger of, the MPT, consistent with coupled ice-sheet–carbon cycle feedback frameworks.

How to cite: Xu, A. and Frank, N.: Strengthened Icelandic Ice Sheet control on Northeast Atlantic neodymium isotope variability across the Mid-Pleistocene Transition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10172, https://doi.org/10.5194/egusphere-egu26-10172, 2026.

EGU26-10519 | ECS | Posters on site | CR2.2

Sub-Ice Shelf Topography in Antarctica: Aerogeophysical Modelling and Implications for Ice Shelf Stability – A Case Study at the Evans Ice Stream 

Laura K. Höppner, Graeme Eagles, Hannes Eisermann, Boris Dorschel, Roland Pail, Wolfram H. Geissler, and Alex M. Brisbourne

The ice sheets of the Antarctic continent are supported and stabilised by floating ice shelves. Any future decrease in ice shelf mass and stability is expected to increase ice sheet drainage thus potentially contributing to a rise in the global sea level. Basal melting is a critical factor concerning ice shelf stability. Its rates are strongly dependent on the bathymetry underneath the ice shelves, as this directly influences sub-ice water circulation and its interactions with the open ocean. Therefore, accurate knowledge of sub-ice bathymetry is crucial to estimate the exchange of water masses and heat with the open ocean. We have created a model of the seafloor topography beneath the Evans Ice Stream - draining into the Ronne Ice Shelf, one of the world’s largest ice shelves - by the inversion of legacy airborne gravity data constrained by seismic and ice-penetrating radar depth references. The new bathymetric model is a distinct improvement over existing topographic compilations based on interpolated depths, providing a range of new information on topographic characteristics beneath the ice shelf with increased resolution and detail. The model shows a deep, asymmetric and U-shaped trough beneath the Evans Ice Stream that follows the ice stream’s flow direction. The bathymetry shows that the retrograde slope of the seafloor on the continental shelf and beneath the outer Ronne Ice Shelf continues as far as the ice stream’s grounding line. Should warm water masses from the open ocean cross the continental shelf edge, this slope would permit intrusion of these water masses all the way up to the grounding line. The new bathymetric model thus enables a step towards being able to more confidentially estimate basal melt rates beneath the Evans Ice Stream and their effect on ice shelf and ice sheet stability. The depth and shape of the seabed beneath numerous other ice shelves and areas of permanent sea ice coverage around the Antarctic margins remains poorly constrained or completely unknown. As well as the Evans cavity model, new data and plans for upcoming bathymetric modelling of some of these other areas are highlighted.

How to cite: Höppner, L. K., Eagles, G., Eisermann, H., Dorschel, B., Pail, R., Geissler, W. H., and Brisbourne, A. M.: Sub-Ice Shelf Topography in Antarctica: Aerogeophysical Modelling and Implications for Ice Shelf Stability – A Case Study at the Evans Ice Stream, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10519, https://doi.org/10.5194/egusphere-egu26-10519, 2026.

EGU26-10967 | ECS | Posters on site | CR2.2

Modeling the Greenland ice sheet and Antarctic ice sheet during the mid-Piacenzian Warm Period 

Jonas Van Breedam and Philippe Huybrechts

The mid-Piacenzian Warm Period (mPWP; 3.264 to 3.025 Ma) is a ~240 kyr long period with CO2 concentrations between 350 and 530 ppmv, in the same range as in the middle of the road emission scenario SSP2-4.5 by 2100. Temperatures were between 2 and 5˚C above the pre-industrial state for a sustained period and as a result, sea-level high stands up to +17.2 m have been inferred. Taking into account a maximum contribution from thermal expansion of 1.6 m, the remainder should have been caused by (partial) melting of either the Greenland ice sheet (GrIS) or the Antarctic ice sheet (AIS), or both, as other ice sheets on the continents of the northern hemisphere were very likely absent.

Previous work has illustrated that the simulated GrIS and AIS size is strongly dependent on the applied climate -and ice sheet models. One way to constrain the ice sheet volume of the GrIS and AIS is by making use of the partition of the benthic oxygen isotope records in a terrestrial ice sheet component and a deep-sea temperature change component. Here we simulate various GrIS and AIS geometries based on available climate model output from the Pliocene Model Intercomparison Phase 2 (PlioMIP2) and compute the isotopic composition of the ice sheets. By selecting the ice sheet geometries that correspond best to the reconstructions for the terrestrial ice sheet component from the benthic oxygen isotope record, we further constrain the minimum GrIS and AIS extent during the mPWP.

How to cite: Van Breedam, J. and Huybrechts, P.: Modeling the Greenland ice sheet and Antarctic ice sheet during the mid-Piacenzian Warm Period, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10967, https://doi.org/10.5194/egusphere-egu26-10967, 2026.

EGU26-11397 | ECS | Posters on site | CR2.2

Extent and Dynamics of the Western Patagonian Ice Sheet Between 16 and 42 kyr cal BP 

Karim Lebeaupin, Sebastien Bertrand, Giuseppe Siani, Elisabeth Michel, Lena Andrzejewski, and Julie Leonetti

During the Last Glacial Maximum, the Patagonian Ice Sheet (PIS) was the second-largest ice mass in the Southern Hemisphere after Antarctica, extending across the southern Andes from ~38°S to 55°S. Today, only 5% of this ice mass remains. Here, we present a continuous reconstruction of the extent and dynamics of the western PIS between 16 and 42 kyr cal BP, derived from marine sediment core MD07-3119. The core was analysed using a multiproxy inorganic approach, including grain size, ice-rafted debris (IRD), inorganic geochemistry, and bulk mineralogy, to reconstruct sediment provenance and transport processes. These results are compared with moraine-based chronologies from the eastern PIS. Variations in bulk mineralogy, IRD content, and inorganic geochemistry indicate that the western PIS, which was land-terminating until 37 kyr cal BP, experienced five distinct Ice Expansion Intervals between 16 and 37 kyr cal BP. Data indicate that each Ice Expansion Interval is associated with enhanced sediment input from the coastal metamorphic unit. Our record indicates periods of high sediment discharge of predominantly Patagonian batholith origin corresponding to melting phases between these advances. The longest advance, at 37–31 kyr cal BP, lasted nearly 6 kyr. Variations in provenance proxies imply that PIS outlet glaciers retreated at least 65 km inland between successive advances. Our reconstruction indicates a complex temporal relationship between the western and eastern PIS margins. Overall, most ice retreat intervals in MD07-3119 match terrestrial exposure ages from the eastern side of the PIS, but the eastern PIS often appears to start shrinking earlier than its western side.

How to cite: Lebeaupin, K., Bertrand, S., Siani, G., Michel, E., Andrzejewski, L., and Leonetti, J.: Extent and Dynamics of the Western Patagonian Ice Sheet Between 16 and 42 kyr cal BP, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11397, https://doi.org/10.5194/egusphere-egu26-11397, 2026.

EGU26-11453 | ECS | Orals | CR2.2

Future Antarctic ice loss under climate overshoot trajectories 

Ann Kristin Klose and Ricarda Winkelmann

Earth’s climate is fast approaching a warming of 1.5°C above pre-industrial levels. While the global mean temperature change may be limited on the long term following an overshoot (or peak-and-decline) climate trajectory, the regional climate impacts in Antarctica that might result are highly uncertain: Given the complex interplay of several amplifying and dampening feedbacks in the Antarctic ice-sheet system and associated tipping dynamics, a rich set of changes – ranging from (fully) reversible to potentially irreversible to irreversible – are possible. 

Here, we quantify the response of the Antarctic Ice Sheet and associated uncertainties across multi-centennial to millennial timescales to a wide range of projected climate overshoot trajectories using the Parallel Ice Sheet Model (PISM). 

Overall, our results suggest that the impacts of overshooting 1.5°C on the Antarctic Ice Sheet worsen with increasing magnitude and duration, and are strongly dependent on the landing climate. Even temporary overshoots can have long-lasting, if not irreversible impacts, stressing the need for limiting global warming to ensure the stability of the Antarctic Ice Sheet across timescales.

How to cite: Klose, A. K. and Winkelmann, R.: Future Antarctic ice loss under climate overshoot trajectories, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11453, https://doi.org/10.5194/egusphere-egu26-11453, 2026.

EGU26-12014 | ECS | Orals | CR2.2

Sources of oceanic and volcanic heat melting a subglacial channel in Kamb Ice Stream,West Antarctica 

Peter Washam, Britney Schmidt, Brice Loose, Huw Horgan, Craig Stewart, Craig Stevens, Justin Lawrence, Christina Hulbe, and Benjamin Hurwitz

Melting from oceanic heat and basal lubrication from subglacial freshwater are fundamental elements of West Antarctic Ice Sheet mass balance that are poorly constrained. The ice streams feeding the Ross Ice Shelf grounding line periodically start and stall over decadal to century timescales due to shifts in these forcings. Here, we present in situ hydrographic measurements, noble gas abundances, and helium isotope ratios from a l a r g e subglacial channel melted into the base of stagnant Kamb Ice Stream. These data identify an outflowing plume containing subglacial freshwater admixture from upstream volcanic activity and anomalously warm inflowing seawater containing Circumpolar Deep Water from the Ross Sea, with oceanic heat delivery outpacing that from volcanism. Our results directly quantify both variables that affect the mass balance of the Ross Ice Shelf’s sensitive interconnected ice streams and highlight the vulnerability of this region of West Antarctica to increased forcing from a warming climate.

How to cite: Washam, P., Schmidt, B., Loose, B., Horgan, H., Stewart, C., Stevens, C., Lawrence, J., Hulbe, C., and Hurwitz, B.: Sources of oceanic and volcanic heat melting a subglacial channel in Kamb Ice Stream,West Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12014, https://doi.org/10.5194/egusphere-egu26-12014, 2026.

EGU26-12182 | ECS | Orals | CR2.2

Seasonal climate impacts on LGM glaciers in the Vosges(France): Insights from GRISLI modeling and paleo-extent 

Gabriel Fénisse, Aurélien Quiquet, Jean-Baptiste Brenner, Pierre-Henri Blard, and David Vincent Bekaert

Glaciers are key hydro-climatic indicators and markers of atmospheric changes in the past, making them essential tools for reconstructing glacial paleoenvironments and paleoclimates. As a climatically stable period that is drastically different from today, the Last Glacial Maximum (LGM, 26–19 ka BP) is widely used as a benchmark for evaluating climate sensitivity (i.e., a key parameter linking atmospheric CO₂ to temperature) and for comparing climate model simulations with continental reconstructions from multiple proxy archives.

Pollen assemblages are a commonly used proxy for reconstructing past temperature changes, as they offer broad spatial coverage across Europe. However, particularly in Europe, simulated LGM annual temperatures often show substantial disagreement with reconstructions and appear highly heterogeneous across models. Dated glacier extents provide an independent archive, helping to assess data–model comparisons.

Temperature is a critical variable to estimate the surface mass balance of glaciers (i.e., the difference between accumulation and ablation). Surface mass balance models (e.g., the positive degree day, PDD, model; [1]) provide the climatic conditions required to reproduce the extent of paleo-ice sheets (inverse approach), as constrained by geomorphological evidence.

PDD-based ice sheet models in central Europe ([2]; [3]) indicate stronger LGM cooling than pollen reconstructions (e.g., [4]), a mismatch likely linked to seasonal biases given the high sensitivity of glaciers to seasonal temperatures ([5]; [6]). Yet, seasonal LGM reconstructions remain scarce, and recent syntheses highlight marked inconsistencies in seasonality anomalies across European glaciated regions, including the Vosges ([7]) - which are too small to be captured by climate models (Global Circulation Models, GCMs).

Using a new compilation of 10Be cosmogenic exposure ages ([8]; [9]) in the Vosges Mountains (NE France) and the GRISLI ice sheet model ([10]), this study investigates the impact of LGM seasonal and precipitation anomalies on simulated glacier extents and on LGM data-model cooling agreement.

As results, we deduce a high variability of LGM climate conditions sufficient to reproduce the paleo-ice sheet extent in the Vosges, yet none of them match the pollen-based paleoclimatic reconstructions ([11]). However, some LGM climate models produce temperature conditions (annual and seasonal) similar to the GRISLI results, while producing lower precipitation in the Vosges (60% to 120% lower than GRISLI results). While the calibration of the GRISLI model has a minor effect on these results, one of the more feasible ways to minimize data–model discrepancies in climate spaces - considering paleoclimatic reconstructions - would be to substantially increase precipitation (+380%, i.e., ~5 times modern precipitation) in the restricted Vosges massif during the LGM.

[1] Reeh, 11-128 (erschienen, 1991)

[2] Allen +, https://cp.copernicus.org/articles/4/249/2008/

[3] Heyman, https://doi.org/10.1016/j.yqres.2012.09.005

[4] Davis +, https://cp.copernicus.org/articles/20/1939/2024/

[5] Oerlemans and Riechert, https://doi.org/10.3189/172756500781833269

[6] Huss and Hock, https://www.nature.com/articles/s41558-017-0049-x

[7 & 11] Fénisse +, in prep

[8] Harmand, https://doi.org/10.4000/rge.9703

[9] Blard +, in prep

[10] Quiquet +, https://doi.org/10.5194/gmd-11-5003-2018

How to cite: Fénisse, G., Quiquet, A., Brenner, J.-B., Blard, P.-H., and Bekaert, D. V.: Seasonal climate impacts on LGM glaciers in the Vosges(France): Insights from GRISLI modeling and paleo-extent, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12182, https://doi.org/10.5194/egusphere-egu26-12182, 2026.

EGU26-12379 | ECS | Orals | CR2.2

Tracing Greenland Ice Sheet dynamics during past warm climates 

Tjördis Störling, Nynke Keulen, Sebastian N. Malkki, Kristine Thrane, Benjamin Heredia, Ricardo D. Monedero-Contreras, Lara F. Perez, Heike H. Zimmermann, and Paul C. Knutz

Understanding the response of the Greenland Ice Sheet to past climate variability is essential for improving projections of its future evolution and contributions to sea-level rise. As part of the ChronIce project (Chronicling Greenland Ice Sheet evolution through past warm climates), this study investigates the response of the northern Greenland Ice Sheet to past climate forcing by reconstructing changes in physical weathering, erosion, and ice–ocean dynamics. We focus on North-West Greenland using a unique marine sedimentary archive recovered during International Ocean Discovery Program Expedition 400.

Temporal variations in glacial outlet provenance, weathering intensity, and erosion are examined using detrital mineralogical and geochemical approaches applied to sediment records from sites U1604, U1606, U1607 and U1608. Heavy mineral fractions are analyzed using Automated Quantitative Mineralogy–Scanning Electron Microscopy (AQM-SEM) and Laser Ablation–Inductively Coupled Plasma–Mass Spectrometry (LA-ICP-MS) that enables single-grain U–Pb geochronology and provenance fingerprints of ice-rafted debris (IRD). Here we will show results from zircon, apatite, titanite, and other datable minerals which, in combination with IRD grain-size and textural analyses, can provide new insights on sediment transport pathways, weathering processes and source regions linked to glacial erosion during the late Pliocene and Pleistocene.  

How to cite: Störling, T., Keulen, N., Malkki, S. N., Thrane, K., Heredia, B., Monedero-Contreras, R. D., Perez, L. F., Zimmermann, H. H., and Knutz, P. C.: Tracing Greenland Ice Sheet dynamics during past warm climates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12379, https://doi.org/10.5194/egusphere-egu26-12379, 2026.

EGU26-12617 | Orals | CR2.2

IPSL-CM-Elmer/Ice: a new coupled ice sheet – climate model 

Lucas Bastien, Pierre Mathiot, Nicolas C. Jourdain, Cécile Agosta, Justine Caillet, Arnaud Caubel, Sylvie Charbit, Mondher Chekki, Julie Deshayes, Christophe Dumas, Gaël Durand, Fabien Gillet-Chaulet, Olivier Marti, Cyrille Mosbeux, and Etienne Vignon

The contribution of ice sheets to future sea level rise remains highly uncertain, and complex positive feedback mechanisms can lead to accelerating melt in a warming climate. Yet, few climate models explicitly represent ice flow of Greenland and Antarctica, or their interactions with the rest of the climate system.

Here we present the coupling of the Elmer/Ice ice sheet model with the IPSL-CM7 climate model. Two-way coupling with the atmospheric and oceanic components of IPSL-CM7 (LMDZ and NEMO, respectively) occurs every simulated year. On the atmospheric side, the surface mass balance from LMDZ is used to force the ice sheet model. In this coupling step, a positive degree day scheme is used to re-calculate surface melt and runoff for Greenland to yield more realistic results. The elevation of the LMDZ domain’s bottom surface is in turn updated to account for the new ice sheet geometry provided by Elmer/Ice. On the ocean side, sub-ice shelf melting is explicitly represented where NEMO's resolution allows it and is extrapolated near the grounding line and under small ice shelves, where the cavity geometry is not resolved by the ocean model. NEMO’s computational domain is updated yearly to account for new icy or wet cells.

We then present the results of two 100-year simulations, which were conducted to test the robustness of the coupling and the behaviour of the model in a warming climate. The first  simulation has a constant pre-industrial atmospheric CO2 concentration, whereas in the second one  the CO2 concentration increases by 1% every year. We describe some interesting features that emerge due to increasing CO2 concentrations, such as the transition from cold to warm water on the continental shelf of the Amundsen Sea, and a retreat of the grounding line in this region.

While still in its early stage of development, this work is an important milestone in the addition of interactive ice sheets within the IPSL-CM7 climate model. Future developments include interactive ice fronts, which are currently fixed in the model, and the possibility of uncovering solid ground as ice sheets retreat.

How to cite: Bastien, L., Mathiot, P., Jourdain, N. C., Agosta, C., Caillet, J., Caubel, A., Charbit, S., Chekki, M., Deshayes, J., Dumas, C., Durand, G., Gillet-Chaulet, F., Marti, O., Mosbeux, C., and Vignon, E.: IPSL-CM-Elmer/Ice: a new coupled ice sheet – climate model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12617, https://doi.org/10.5194/egusphere-egu26-12617, 2026.

EGU26-13478 | Posters on site | CR2.2

Antarctic Ice Sheet response over the next 10,000 years: ice sheet dynamics interacting with solid Earth deformations and sea-level change 

Seyedhamidreza Mojtabavi, Torsten Albrecht, Matteo Willeit, Nellie Wullenweber, Reyko Schachtschneider, and Volker Klemann

Antarctica has the largest potential contribution to sea-level change within the modern cryosphere. Therefore, reliable predictions of future sea-level change from the Antarctic Ice Sheet are crucial. Ice sheet interactions with other Earth system components are crucial for making accurate predictions of sea-level change, as relevant interactive feedbacks can amplify or dampen the anthropogenic induced effects and affect associated response time scales. In most ice sheet model projections so far, models generally assume constant bed topography and sea level. Neglecting the stabilizing sea-level feedback due to glacial isostatic adjustment (GIA), i.e., gravitationally, rotationally, and deformationally (GRD) consistent deformations of the solid Earth and sea level change, tends to overestimate the Antarctic Ice Sheet’s contribution to sea level rise on centennial timescales, particularly in regions with very low mantle viscosities and a thin lithosphere. 

 

As part of the PalMod project, we present first results of multi-millennial future simulations with the interactively coupled Parallel Ice Sheet Model (PISM), which represents ice sheet dynamics, together with two glacial isostatic adjustment (GIA) models of different complexity: VILMA (VIscoelastic Lithosphere and MAntle model) and the Lingle–Clark (LC) model. For climatic forcing, we used surface temperature and surface mass balance from the regional climate model RACMO, forced by the climate model CESM2-WACCM, while long-term climate evolution was taken from CLIMBER-X. VILMA is applied as a global GIA model that captures all GRD components and accounts for the 3-dimensional Earth structure. The LC model, which is often used in ice sheet modelling, represents a regional viscoelastic GIA model with constant values for upper-mantle viscosity and lithosphere thickness and only accounts for vertical land motion. The simulations cover the period from the pre-industrial era up to the year 10,000. The projections assess the influence of different Earth structures on ice sheet mass changes, which we show result in particularly different trajectories on the longer time scales.

How to cite: Mojtabavi, S., Albrecht, T., Willeit, M., Wullenweber, N., Schachtschneider, R., and Klemann, V.: Antarctic Ice Sheet response over the next 10,000 years: ice sheet dynamics interacting with solid Earth deformations and sea-level change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13478, https://doi.org/10.5194/egusphere-egu26-13478, 2026.

EGU26-14169 | ECS | Orals | CR2.2

Glacial processes and sediment provenance in basal ice, subglacial and fluvial sediments from Greenland: insights from mineralogy, grain morphology, and isotopic analyses 

Louise Crinella Morici, Pierre-Henri Blard, Charlotte Prud'Homme, Yves Marrocchi, Marek Stibal, Petra Klímová, Charlotte Skonieczny, Maxime Leblanc, William C Mahaney, Nicolas Perdrial, Catherine Zimmermann, Lisa Ardoin, Jean-Louis Tison, Jørgen Peder Steffensen, François Fripiat, Anders Svensson, and Dorthe Dahl-Jensen

The accelerated melting of the Greenland Ice Sheet is one of the consequences of current global warming. In addition to being affected by Arctic amplification, Greenland could contribute dramatically to future sea-level rise. However, our current knowledge of the evolution of the Greenland Ice Sheet (GrIS) during the warmest periods of the Quaternary, as well as of subglacial geology and geochemistry, remains limited, notably due to the scarcity of available basal ice and subglacial sediment samples. Within the framework of the ERC Green2Ice project, we present preliminary results from the analysis of basal ice and subglacial sediments from the Camp Century ice core (1966, northwestern Greenland, 1388 m depth beneath the ice sheet, frozen bed). For comparison, we also studied samples collected from different glacio-geological settings in the Kangerlussuaq region (western margin of Greenland): (i) a subglacial drilling sample (H1-1, 1250 m depth, temperate bed) and (ii) a sediment sample from the Kangerlussuaq River. Morphological, mineralogical, and isotopic analyses were conducted to characterize the geological and geochemical nature of the debris, their provenance, and the sequence of processes recorded, such as deglaciation phases and subglacial weathering. Six samples (four from the Camp Century basal sediment section, one from the Kangerlussuaq River, and one from the H1-1 drill) with grain sizes ranging from 125 µm to 2 mm were analysed using Scanning Electron Microscopy (SEM) coupled with Energy-Dispersive Spectroscopy (EDS). Grain morphologies observed under SEM reflect different transport modes (glacial, fluvial, aeolian), allowing the identification of local phases of ice-sheet retreat and advance. EDS provides information on grain mineralogy, notably the presence of clay coatings, which are indicative of stable, ice-free environmental conditions. The clay fraction of the basal and subglacial ice from Camp Century, as well as that of H1-1 and the Kangerlussuaq River, was analysed by X-ray Diffraction, providing information on the different clay mineral species present, some of which indicate deglaciation conditions. Finally, the isotopic ratio 87Sr/86Sr and ɛNd of Camp Century samples and those from the Kangerlussuaq region constrain the provenance of the debris. The morphological and mineralogical analyses reveal (i) distinct geological source areas depending on location and (ii) a complex grain history combining sedimentary transport and weathering phases during ice free conditions. 87Sr/86Sr and ɛNd isotopic analyses from the silicates of the basal and subglacial ice samples will provide further constrains on the source materials, this constraint being notably key to assess the origin of the clay fraction in the silty ice of Camp Century, and in the intermediate ice rich unit with the basal sedimentary section.

How to cite: Crinella Morici, L., Blard, P.-H., Prud'Homme, C., Marrocchi, Y., Stibal, M., Klímová, P., Skonieczny, C., Leblanc, M., Mahaney, W. C., Perdrial, N., Zimmermann, C., Ardoin, L., Tison, J.-L., Steffensen, J. P., Fripiat, F., Svensson, A., and Dahl-Jensen, D.: Glacial processes and sediment provenance in basal ice, subglacial and fluvial sediments from Greenland: insights from mineralogy, grain morphology, and isotopic analyses, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14169, https://doi.org/10.5194/egusphere-egu26-14169, 2026.

EGU26-14253 | ECS | Posters on site | CR2.2

Exploring Earth System Model Forcings for Ice Sheet Tipping Point Experiments in TIPMIP-ICE 

Leonie Röntgen, Ann Kristin Klose, Torsten Albrecht, Jorge Bernales, Chuncheng Guo, Klaus Wyser, Robin S. Smith, Christine Hvidberg, Shuting Yang, and Ricarda Winkelmann

The Tipping Points Modelling Intercomparison Project (TIPMIP) uses Earth System models (ESMs) and stand-alone models to assess tipping point risks. Within TIPMIP-ICE, stand-alone ice sheet models are forced with temporally extended atmospheric and oceanic output from multiple TIPMIP ESMs, making the choice of forcing a critical source of uncertainty.

We explore TIPMIP ESM results in Antarctica for the historical period as well as under positive and zero emission scenarios to (1) decide on suitable forcing data for ice sheet simulations and to (2) understand simulated ice sheet changes in relation to the ESM forcing. The analysis focuses on ocean potential temperature and salinity at the Antarctic continental shelf depth, near-surface air temperature, and precipitation as key fields for sub-shelf melt, surface mass balance, and ice sheet stability. It includes a comparison to observations and an assessment of multi-model differences under positive and zero emissions scenarios. 

Comparing historical runs (1981-2010) to observations reveals oceanic temperature biases across the ESMs of up to +4°C/-2°C. Under an idealized positive emission experiment to +2°C of global mean warming, preliminary results show spatial variability across basins in Antarctica. Different models follow distinct atmosphere-ocean warming trajectories, resulting in different forcing patterns for ice sheet models. 

These distinct warming trajectories could impact the risk of ice sheet tipping dynamics in TIPMIP-ICE, particularly the grounding-line stability of Antarctica. They underline the importance of having a diverse set of ESM forcings to enable future evaluation of  feedbacks associated with tipping dynamics of the ice sheets such as melt-elevation feedback or marine ice sheet instability (MISI). Ongoing work extends this analysis to additional ESMs and to Greenland.

How to cite: Röntgen, L., Klose, A. K., Albrecht, T., Bernales, J., Guo, C., Wyser, K., Smith, R. S., Hvidberg, C., Yang, S., and Winkelmann, R.: Exploring Earth System Model Forcings for Ice Sheet Tipping Point Experiments in TIPMIP-ICE, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14253, https://doi.org/10.5194/egusphere-egu26-14253, 2026.

EGU26-14288 | Orals | CR2.2

Long-term future Greenland ice loss determined by peak global warming 

Matteo Willeit, Alexander Robinson, Christine Kaufhold, and Andrey Ganopolski

The Greenland ice sheet (GrIS) is recognised as highly sensitive to climate change, with palaeoclimate evidence and modellingstudies suggesting that sustained global warming only marginally above present-day levels could trigger its complete deglaciation over multi-millennial timescales. Despite growing understanding of threshold behaviour in the GrIS, the implications of a temporal crossing of this temperature threshold, particularly the duration and magnitude of temperature overshoots, for the future GrIS mass loss trajectory remain poorly constrained. Here we present simulations of the next 10,000 years under a range of future anthropogenic emissions scenarios, performed using a fully coupled Earth system model with a dynamic GrIS and interactive atmospheric CO2 and CH4. Our model experiments span scenarios from strong mitigation to high emissions SSP pathways, allowing systematic exploration of the relationship between warming trajectories and ice sheet response.
We find that the long-term ice loss on Greenland is predominantly determined by the peak global temperature increase relative to pre-industrial levels, which generally occurs within the next few centuries depending on the emissions pathway. The GrIS contribution to global mean sea-level rise after 10,000 years increases by approximately 2 metres for each degree of warming above a critical peak global warming threshold of approximately 2°C above pre-industrial temperatures, which is close to the GrIS equilibrium tipping point. This finding is robust for different equilibrium climate sensitivities and across different scenarios. Furthermore, when accounting for variations in the Earth's orbital parameters over the next 10,000 years, the sensitivity of the GrIS mass loss to anthropogenic warming substantially increases, as future orbital configurations lead to higher summer insolation over Greenland.
Overall, our results demonstrate how 21st century climate policy will largely determine the fate of the GrIS for millennia to come.

How to cite: Willeit, M., Robinson, A., Kaufhold, C., and Ganopolski, A.: Long-term future Greenland ice loss determined by peak global warming, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14288, https://doi.org/10.5194/egusphere-egu26-14288, 2026.

EGU26-14389 | ECS | Orals | CR2.2

Mass loss reversibility of the West Antarctic Ice Sheet 

Daniel Moreno-Parada, Violaine Coulon, and Frank Pattyn

Over the last two decades, the contribution of the West Antarctic Ice Sheet (WAIS) to sea level rise (SLR) has doubled. Current observations show that grounding-line retreat is highly discontinuous and strongly modulated by ocean variability, with the strength and timing of decadal extremes exerting a greater influence than long-term mean changes. Here, we analyse the future behaviour of the WAIS by incorporating multiple random realizations of plausible climate scenarios in Kori-ULB ice-sheet model simulations. We further develop a statistically robust metric to assess grounding line stability in a spatial context, not only in the time domain as currently expressed in terms of SLR uncertainties. We thus define a “safety band" as the location where grounding line retreat is still reversible. Beyond this band, glaciers undergo a self-sustained retreat irrespective of ambient climate conditions. On the contrary, grounding lines that remain within this band still allow for glacier slowdown and even re-advance in the absence of ocean melt or if sub-shelf accretion occurs. The window for effective climate mitigation therefore remains open only while the grounding line stays within this safety band. Our results provide a robust metric for assessing glacier stability and highlight the need to account for climate variability in sea-level rise projections.

How to cite: Moreno-Parada, D., Coulon, V., and Pattyn, F.: Mass loss reversibility of the West Antarctic Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14389, https://doi.org/10.5194/egusphere-egu26-14389, 2026.

EGU26-15767 | ECS | Orals | CR2.2

Multiphase glaciations in East Siberia during the late Quaternary revealed by Arctic zircon U-Pb ages 

Han Feng, Zhengquan Yao, Xuefa Shi, Zhongshi Zhang, Huayu Lu, Hanzhi Zhang, Yanguang Liu, Xin Shan, Jiang Dong, Linsen Dong, Gongxu Yang, Limin Hu, Yuri Vasilenko, Anatolii Astakhov, and Alexander Bosin

The Northern Hemisphere ice sheets have undergone significant periodic changes during the Quaternary. These changes not only influence global sea-level fluctuations but also drive global climate evolution. Consequently, reconstructing the evolution of these ice sheets has been a key objective in Earth science. Over recent decades, tracking the sources of ice-rafted debris (IRD) in the Arctic Ocean's deep-sea sediments has enabled researchers to systematically reconstruct the histories of the North American and Eurasian ice sheets. However, due to the lack of diagnostic provenance tracers specific to the East Siberian Ice Sheet, its evolution remains highly controversial. To address this gap, we conducted a provenance analysis based on a comprehensive detrital zircon U-Pb age dataset. This dataset comprises 10,111 new ages from both surface sediments on the circum-Arctic shelves and IRD in deep-sea cores from the central Arctic Ocean. Our results reveal distinct zircon age distributions across different circum-Arctic shelf regions. Notably, a prominent age peak at ~90–110 Ma serves as a diagnostic fingerprint for sediments derived from the East Siberian continent and shelf. Central Arctic Ocean sediments from at least four glacial intervals contain coarse zircon grains bearing this diagnostic ~90–110 Ma peak, strongly indicating iceberg transport from East Siberia. This implies that the East Siberian continent and shelf experienced multiple glaciations, likely within the past three glacial-interglacial cycles. The repeated glaciation of East Siberia likely exerted significant, though still poorly quantified, influences on both polar and global climates during the late Quaternary. Our findings provide new insights into the history of Northern Hemisphere glaciation and propose a valuable approach for reconstructing ice sheet evolution.

How to cite: Feng, H., Yao, Z., Shi, X., Zhang, Z., Lu, H., Zhang, H., Liu, Y., Shan, X., Dong, J., Dong, L., Yang, G., Hu, L., Vasilenko, Y., Astakhov, A., and Bosin, A.: Multiphase glaciations in East Siberia during the late Quaternary revealed by Arctic zircon U-Pb ages, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15767, https://doi.org/10.5194/egusphere-egu26-15767, 2026.

EGU26-16180 | Orals | CR2.2

Shallow geology of the sub-ice-shelf Siple Coast, eastern Ross Sea, Antarctica constrained by reflection seismology and surface gravity surveying 

Andrew Gorman, Matthew Tankersley, Jenny Black, Huw Horgan, Gary Wilson, and Gavin Dunbar

The geological units underlying the grounding line between the West Antarctic Ice Sheet and the Ross Ice Shelf are expected to contain a record of repeated ice advance and retreat in a key area for understanding interactions between the ice sheet, the ocean and the solid Earth through the warm and cold periods of the Quaternary. Direct sampling of the sedimentary units in the vicinity of the grounding line across the relatively slow-moving Kamb Ice Stream has been an ongoing focus for drilling efforts that involve first melting through roughly 600 m of ice. Geophysical methods suggest that the region is underlain by a sedimentary basin of yet-to-be-determined thickness.  However, little is yet known about sediment lithology and stratigraphy in this region.

We present analysis of a grid of about 73 km of seismic reflection profiles collected in the Kamb Ice Stream grounding line region during three seasons since early 2015, integrated with the inversion of a grid of surface-collected gravity data. Seismic data were acquired with explosive charges frozen into shallow (mostly 25-m-deep) hot-water-drilled holes recorded by surface-deployed geophones buried in the firn. Seismic processing has been undertaken to maximise resolution of stratigraphic units at and below the sea floor. The inversion of coincident surface-based gravity data, integrated with airborne-gravity collected as part of the ROSETTA-Ice project, constrains basin thickness in the region of the seismic data.

The processed low-fold seismic data image the ice shelf, ocean cavity and underlying stratigraphy. The shallow stratigraphy appears to be mostly horizontally layered, typical of a sub-ice continental shelf environment. More than 300 m of sub-horizontally layered sedimentary strata can be identified above the first inter-ice multiple reflection in the data. Several distinct reflections interpreted as unconformities are identified in the seismic data, which combined with reflective characteristics, terminations and pinchouts enable a seismic stratigraphic interpretation to be undertaken. For example, unconformities between units could correspond to past glacial erosion episodes as the position of the grounding line in this region has migrated toward or away from the open ocean. The integration of surface and airborne gravity data here enables better constrained modelling of the thickness of the sedimentary basins in the region that cannot be imaged by the seismic reflection data.

How to cite: Gorman, A., Tankersley, M., Black, J., Horgan, H., Wilson, G., and Dunbar, G.: Shallow geology of the sub-ice-shelf Siple Coast, eastern Ross Sea, Antarctica constrained by reflection seismology and surface gravity surveying, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16180, https://doi.org/10.5194/egusphere-egu26-16180, 2026.

EGU26-16956 * | Orals | CR2.2 | Highlight

Modelling Ice-Sheet Contributions to Sea Level: Progress, Uncertainty, and Outlook 

Gael Durand and Cyrille Mosbeux

Ice sheets play a central role in the Earth system: they regulate global sea level, influence ocean circulation through freshwater fluxes, and interact with the atmosphere via albedo and elevation feedbacks. Over recent decades, both the Greenland and Antarctic ice sheets have been losing mass at an accelerating rate, making them an increasing contributor to observed sea-level rise. This mass loss will continue throughout the 21st century and beyond. Yet, despite major advances in observations and modelling, projections of future ice-sheet mass loss remain affected by deep uncertainties, arising from complex ice dynamics, poorly constrained boundary conditions, and nonlinear interactions with the climate system.

This talk provides a synthesis of recent progress in ice-sheet modelling, with a focus on developments that have reshaped our ability to simulate past and future ice-sheet evolution. We review advances in the representation of key physical processes, including grounding-line dynamics, basal friction, ice–ocean interactions beneath ice shelves, and damage and calving. We then discuss progress in coupling ice-sheet models with atmosphere and ocean models, ranging from improved offline forcings to emerging fully coupled Earth system frameworks, as well as the growing role of coordinated multi-model ensembles and their analysis in characterising uncertainty and identifying robust responses. We conclude by discussing ice-sheet predictability, showing how present-day observations can provide meaningful constraints on future evolution in specific regions, while informing where and why such constraints are not emerging elsewhere.

How to cite: Durand, G. and Mosbeux, C.: Modelling Ice-Sheet Contributions to Sea Level: Progress, Uncertainty, and Outlook, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16956, https://doi.org/10.5194/egusphere-egu26-16956, 2026.

EGU26-17308 | ECS | Posters on site | CR2.2

Timing and drivers of Patagonian Ice Sheet variability during the last glacial cycle 

Andrés Castillo-Llarena, Matthias Prange, and Irina Rogozhina

During the Last Glacial Maximum (23,000 to 19,000 years ago), the Patagonian Ice Sheet (PIS) covered much of the southern Andes between 38°S and 55°S, representing the largest ice mass in the Southern Hemisphere mid-latitudes. Geological evidence from Patagonia and New Zealand indicates that maximum ice extent was not synchronous with Northern Hemisphere ice-sheet evolution. Here we present transient numerical simulations of the Patagonian Ice Sheet spanning the entire Last Glacial Cycle.

Our results reveal two major phases of ice-sheet expansion, during Marine Isotope Stage 4 and late Marine Isotope Stage 3, superimposed by pronounced inter-millennial-scale variability. These high-frequency fluctuations are consistent with Southern Hemisphere climate variability and exerted a first-order control on the timing and magnitude of ice advances, particularly during intermediate glacial states. Long-term evolution of the PIS is closely linked to changes in integrated summer insolation. This metric combines summer duration and insolation intensity and exhibits an obliquity-like periodicity. This forcing provides a robust explanation for the timing and magnitude of major ice advances. We further suggest that integrated summer insolation played a broader role in modulating glacier behaviour across the Southern Hemisphere mid-latitudes, offering a unifying framework to interpret asynchronous glacial variability between hemispheres.

How to cite: Castillo-Llarena, A., Prange, M., and Rogozhina, I.: Timing and drivers of Patagonian Ice Sheet variability during the last glacial cycle, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17308, https://doi.org/10.5194/egusphere-egu26-17308, 2026.

EGU26-18304 | ECS | Orals | CR2.2

The Role of a Dynamic Greenland Ice Sheet in Future Climate: Insights from Multi-Centennial Coupled UKESM Simulations 

Yiliang Ma, Robin Smith, Steve George, Charlotte Lang, Inès Otosaka, and Dan Hodson

The Greenland Ice Sheet (GrIS) holds an ice volume equivalent to ~7 m of global sea-level rise, making its future evolution a critical component of sea-level projections. The rate and magnitude of ice loss strongly depend on ice–climate feedbacks, yet most Earth System Models (ESMs) still treat ice sheets as static entities, limiting their ability to simulate these essential interactions. The UK Earth System Model (UKESM) is a state-of-the-art ESM which includes dynamic models of the Greenland and Antarctic ice sheets, as well as a sophisticated climate - ice sheet coupling based on the explicit exchanges of water and energy. However, the impacts of this interactivity on projected climate and ice sheet evolution remain insufficiently quantified.

To assess the role of ice–climate feedbacks within a sophisticated, coupled ESM framework, we performed two multi-century climate simulations under high-emissions forcing (SSP5–8.5) using UKESM: a control run with a fixed GrIS geometry, and an interactive run in which the ice sheet evolves freely in response to climate drivers. For computational efficiency, an ice sheet acceleration mode was applied from 2100 onward, whereby the ice sheet model integrates ten years for each year of atmospheric-oceanic simulation. This method effectively projects the ice sheet’s evolution over two millennia (2100–4100) within a 200-year atmosphere-ocean simulation (2100–2300), although it does not fully include feedbacks from meltwater-driven changes in ocean circulation.

By comparing these simulations, we quantify the impacts of simulating a dynamic GrIS in the Earth System, ranging from local alterations in Greenland’s mass balance and sea-level contribution to remote downstream effects on atmospheric circulation. We identify that positive feedbacks—primarily from reduced surface albedo and lowering ice sheet elevation—become dominant after 2100, driving accelerated mass loss and influencing North Atlantic atmospheric circulation patterns. This study highlights the importance of two-way ice–climate coupling in ESMs for improving predictions of future climate and sea level changes.

How to cite: Ma, Y., Smith, R., George, S., Lang, C., Otosaka, I., and Hodson, D.: The Role of a Dynamic Greenland Ice Sheet in Future Climate: Insights from Multi-Centennial Coupled UKESM Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18304, https://doi.org/10.5194/egusphere-egu26-18304, 2026.

EGU26-18694 | Orals | CR2.2

Reconstruction of the late Vistulian Fennoscandian Ice Sheet - based on numerical modelling and sensitivity analyses  

Jakub Zbigniew Kalita, Stewart Jamieson, Caroline Clason, Izabela Szuman, Berit Hjelstuen, Andy Aschwanden, and Maciej Prill

This study presents a modelled reconstruction of the past ice dynamics of the Fennoscandian Ice Sheet, paying particular attention to the interactions between the ice sheet margin in Poland and the Baltic and Norwegian Channel Ice Streams. The focus is on the Late Vistulian time period, 24 – 12 ka BP, a key stage of the Last Glacial Period, characterized by significant climatic fluctuations and a dynamic evolution of the ice sheets over Northern Europe. In our reconstruction we use a numerical model constrained by empirical data, such as glacial landforms, glacial and postglacial deposits, and geochronology, to test the relationship between the modelled extent of the Fennoscandian Ice Sheet and its climatic and basal boundary conditions. A series of simulations were carried out for the Fennoscandian and British–Irish ice sheets with a spatial resolution of 10 km. These simulations applied and modified climates from the Paleoclimate Modelling Intercomparison Project – Phase 4 (PMIP4), and in tandem explored the importance of basal friction conditions on ice behaviour in this region. The modelling results reveal the existence of ice streams with diverse spatiotemporal characteristics. Their widths range from several tens to several hundreds of kilometres, while velocities vary from a few hundred to more than 1000 meters per year. The dynamic behaviour of these ice streams strongly controls the southern extent of the Fennoscandian Ice Sheet during deglaciation, forming pronounced lobate outlets reaching several hundred kilometres in length and several hundred meters in thickness at the Southern margin. Significantly, adjustments impacting friction beneath one ice stream alters its behaviour in such a way that it then influences the dynamics of other ice streams. In particular, there is a significant interplay such that when we reduce activity of Norwegian Channel Ice Stream, the ice divide between the Baltic Ice Stream and the Norwegian Channel Ice Stream migrates. As a consequence, this changes the behavior of Baltic Ice Stream and the extent of the ice at the ice sheet margin in Poland. This is the first time the two major outlets of the Fennoscandian Ice Sheet have been shown to be so strongly linked in controlling the wider southern margin of the ice sheet.

Funding sources: This research was funded by the National Science Centre (NCN) under grant no. 2024/08/X/ST10/00193 and 2015/17/D/ST10/01975.
 
Acknowledgements: Numerical analyses were carried out using the computing cluster provided by the Faculty of Mathematics and Computer Science, Adam Mickiewicz University, Poznań, Poland.

How to cite: Kalita, J. Z., Jamieson, S., Clason, C., Szuman, I., Hjelstuen, B., Aschwanden, A., and Prill, M.: Reconstruction of the late Vistulian Fennoscandian Ice Sheet - based on numerical modelling and sensitivity analyses , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18694, https://doi.org/10.5194/egusphere-egu26-18694, 2026.

Record-shattering climate extremes are becoming a seemingly everyday reality across the globe as anthropogenic climate change accelerates. Over polar regions, similar weather extremes receive less attention, but are responsible for a recent pause and slight reversal of Antarctic ice loss since 2020 and ultimately mitigating global sea-level rise. In March 2022, one particularly extreme weather event in the form of an atmospheric river (AR) caused enough snowfall in East Antarctica to help make 2022 a positive mass year for Antarctica. Yet, this same event caused a heatwave that led to the highest temperature anomaly ever recorded globally (39° C) and triggered the final collapse of the Conger ice shelf simultaneously demonstrating the opposing yet significant effects of extreme weather on the Antarctic mass balance.

While the gradual thinning and grounding line retreat of ice shelves through ocean basal melting pushes ice shelves towards non-viability and collapse in a bifurcation-induced tipping point, extreme weather may trigger that collapse sooner through noise-induced tipping. However, short-medium term (10-50 years) increases in extreme snowfall events may mitigate  ice loss more strongly than currently observed. Thus, to constrain future sea-level rise projections, the potential impacts from extreme weather in the short-medium term must be considered.

The uncertainty in predicting the influence of extreme weather on ice shelf stability is partly due to our limited ability to simulate many of the smaller scale processes and impacts that are essential to fully explain polar extreme weather in the present day combined with a limited understanding of how future changes in extreme weather patterns will influence ice sheet dynamics. Global climate models generally lack the spatial resolution to capture small-scale extreme weather processes, and evaluating their impact on ice sheet dynamics requires coupling to ice sheet models that is currently undeveloped.  

In this talk, I will present the role of extreme weather in influencing the Antarctic mass balance and how extreme weather represents a potential climate tipping point for ice shelf stability. This will involve discussing the current state of Antarctic extreme weather research along with the uncertainties and research gaps in determining the extreme weather risk to ice shelf stability.

How to cite: Wille, J.: Understanding extreme weather risks to ice-sheet stability as a potential climate tipping point, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19541, https://doi.org/10.5194/egusphere-egu26-19541, 2026.

EGU26-20275 | ECS | Orals | CR2.2

European Alpine ice-field dynamics in context of past rapid climate change 

Jean-Baptiste Brenner, Aurélien Quiquet, Didier Roche, and Didier Paillard

Ice-sheet and glaciers constitute an essential component of the climate system and the main storage of freshwater on Earth. Regions particularly sensitive to climate change, the nature and magnitude of their responses to anthropogenic disturbances remain largely uncertain despite the associated challenges (melting ice and reduction of Earth's albedo, contribution to sea level rise, modifications of the oceanic circulation, etc.). In this context, studying the response of the cryosphere to past climate change can give valuable insights about its future evolution. The rapid temperature variations that occurred during the last glacial period are of specific interest for this purpose.

The Late Pleistocene (129-12 ky BP) is indeed marked by abrupt climate oscillations between relatively cold (stadial) and warm (interstadial) conditions in the Northern Hemisphere occurring at millennial time scale. These Dansgaard-Oeschger cycles (D-O) are responsible for strong sub-orbital climate variability, typically about 50% of glacial-interglacial amplitude in Greenland temperature (1). Although the driving mechanisms of D-O remain unclear, changes in the Atlantic Meridional Overturning Circulation are usually invoked for explaining these events, with oscillations between strong and weak transport modes (occurring either spontaneously or in response to external forcing (2)).

Our work analyse the European Alps ice field dynamics in response to rapid climate perturbations during the last glacial cycle. Most modelling experiments on this region focus on the reconstruction of the ice-sheet extent during the Last Glacial Maximum, but studies on the impact of D-O like events are less common. Following an approach tested over the Northern Hemisphere (3), we force the ice-sheet model GRISLI over the Alps during Marine Isotope Stage 3 (60-27 ky BP) with downscaled Paleoclimate Modelling Intercomparison Project climate data. Using two indexes, associated with orbital and millennial-scale variability and respectively applied to i) an Interglacial-LGM anomaly field ii) an AMOC with and without freshwater flux anomaly field, the method allows to take into account the different spatial patterns resulting from orbital and millennial climate fluctuations. The gap between the spatial resolutions of the Global Climate Models simulations and GRISLI is bridged using the downscaling model GeoDS, based on topographical and large scale circulation information.

 

 

(1) Wolff et al. (2010) https://doi.org/10.1016/j.quascirev.2009.10.013

(2) Li and Born (2019) https://doi.org/10.1016/j.quascirev.2018.10.031

(3) Banderas et al. (2015) https://doi.org/10.5194/gmd-11-2299-2018

(4) Brenner et al. (preprint) https://doi.org/10.5194/egusphere-2025-3617

How to cite: Brenner, J.-B., Quiquet, A., Roche, D., and Paillard, D.: European Alpine ice-field dynamics in context of past rapid climate change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20275, https://doi.org/10.5194/egusphere-egu26-20275, 2026.

EGU26-20859 | Posters on site | CR2.2

Climatic proxy based statistical reconstruction of European Ice Sheet for period of 0 to 800 ka 

Izabela Szuman, Jakub Zbigniew Kalita, Leszek Marks, Dariusz Wieczorek, and Lucyna Wachecka-Kotkowska

This study presents European Ice Sheet reconstruction for the period of 0 to 800 ka BP. The model is based on linear regression of 65oN summer insolation, CO2 and the LR04 benthic δ¹⁸O stack fitted to relatively well reconstructed extents of European Ice Sheet during the Vistulian. We tested more than 30 million proxy combinations by scaling and time-shifting the predictors, and selected the best-performing variant using a least-squares criterion. The extrapolation for best combination, resulted in area time series over 800 ka period. The model shows strong relationship between European Ice Sheet area and 65oN summer insolation. Following the insolation signal, the potential for European Ice Sheet to expand and decay is higher than for global trend reflected by global ice volume proxies (i.e. LR04), leading to at least 16 fluctuations where ice sheet area reached area similar MIS2 values, including advances during global interglacial periods (e.g. during MIS7).The European Ice Sheet area during Early (MIS5d, MIS5b) and Middle Vistulian (MIS4) advances is on the same level as during Late Vistulian (MIS2). However, distribution of ice between Kara-Barents, Fennoscandian and British-Irish ice sheets differs and is asynchronous across the Vistulian. We examine this relationship and propose strategy to distribute the total European Ice Sheet area among these regions. Our study enables European Ice Sheet reconstruction trough computationally efficient model. We present a computationally efficient model for reconstructing the European Ice Sheet, enabling analysis of key climatic forcing drivers and better integration with the Earth’s climate system.

 

Funding sources: This research was funded by the National Science Centre (NCN) under grant no. 2024/08/X/ST10/00193 and 2015/17/D/ST10/01975.

 

How to cite: Szuman, I., Kalita, J. Z., Marks, L., Wieczorek, D., and Wachecka-Kotkowska, L.: Climatic proxy based statistical reconstruction of European Ice Sheet for period of 0 to 800 ka, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20859, https://doi.org/10.5194/egusphere-egu26-20859, 2026.

EGU26-21588 | Orals | CR2.2

Antarctic Ice Sheet tipping in the last 800,000 years warns of future ice loss 

David Chandler, Petra Langebroek, Ronja Reese, Torsten Albrecht, Julius Garbe, and Ricarda Winkelmann

Ice loss from the Antarctic Ice Sheet could threaten coastal communities and the global economy if ice volume decreases by just a few percent. Observed changes in ice volume are limited to a few decades, and hard to interpret in the context of an ice sheet with response timescales reaching centuries to millennia. To gain a much longer-term perspective, we combine transient and equilibrium simulations of the Antarctic Ice Sheet response to glacial-interglacial warming and cooling cycles over the last 800,000 years. We find hysteresis between ice volume and climate forcing, caused by the crossing of tipping points as well as the long response time. Notably, West Antarctic Ice Sheet collapse contributes over 4 m sea level rise in equilibrium ice sheet states with little (0.25°C) or even no ocean warming above present. Given that climate projections indicate continued Southern Ocean warming, we will likely cross the threshold for West Antarctic Ice Sheet tipping in the coming decades (if not already). This supports other recent studies warning of substantial irreversible ice loss with little or no further climate warming.

How to cite: Chandler, D., Langebroek, P., Reese, R., Albrecht, T., Garbe, J., and Winkelmann, R.: Antarctic Ice Sheet tipping in the last 800,000 years warns of future ice loss, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21588, https://doi.org/10.5194/egusphere-egu26-21588, 2026.

EGU26-767 | ECS | Posters on site | CR2.3

Seasonal evolution of supraglacial lakes in Northeast Greenland 

Gopika Das K, Saurabh Vijay, and Sushil Kumar Singh

Supraglacial lakes form seasonally on the Greenland Ice Sheet (GIS) during the melt season as surface meltwater accumulates in topographic depressions. These lakes are dynamic, rapidly draining through supraglacial channels or discharging via hydrofractures, contributing to surface runoff and triggering cascading drainage of nearby lakes. Quantifying the spatial and temporal variability of their area, depth and drainage patterns is critical for understanding GIS hydrology and their role in modulating ice sheet behavior. Here we present a quantitative comparison of supraglacial lake evolution and rapid drainage cascade dynamics between contrasting melt years on Northeast Greenland Ice Stream. We analyzed Sentinel-2 observations from the 2019 and 2020 melt seasons using an automated Otsu thresholding approach combining dual water indices such as NDWIice and NDWIGN with topographic depressions from ArcticDEM to map the lakes. Lake depths and volumes were estimated using an empirical relationship between Sentinel-2 reflectance and lake depth calibrated with ICESat-2 ATL03 photon altimetry. We identified rapid drainage events and quantified their spatial and temporal clustering into cascade sequences.

The analysis revealed distinct interannual contrasts in the timing, persistence, and areal extent of supraglacial lakes, reflecting the influence of seasonal temperature variability. In 2019, warmer conditions favored more sustained lake development and prolonged persistence, whereas cooler conditions of 2020 year led to a more rapid rise-and-fall pattern with reduced total storage. Lake formation exhibited a clear elevation dependence, initiating earlier at lower elevations and progressing upward as the melt season advanced. Mid-elevation zones such as  800 to 1000m acted as key reservoirs storing 80% of the total lake volume, hosting the most persistent and voluminous lakes, suggesting their importance in surface-to-bed meltwater routing. Rapid drainage events were different between years despite similar lake inventories. A total of approximately 600 drainage events were identified across both years. Among these approximately 30% of drainage events participated in cascades. Rapid drainage events were concentrated at lower elevations typically below 800m, with a substantial proportion occurring as part of cascading drainage sequences.
Overall, our results demonstrate that variations in melt-season intensity could modulate supraglacial lake persistence, drainage behavior, and cascading dynamics. These findings emphasize the importance of mid-elevation lakes as critical nodes in meltwater transfer and provide new insights into understanding of surface lake water storage and surface-to-bed hydrological connectivity across the NEGIS sector.

How to cite: Das K, G., Vijay, S., and Singh, S. K.: Seasonal evolution of supraglacial lakes in Northeast Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-767, https://doi.org/10.5194/egusphere-egu26-767, 2026.

EGU26-1960 | Orals | CR2.3

Seismic observations reveal a hard-bedded drained subglacial lake basin beneath Isunnguata Sermia, West Greenland  

Adam Booth, Siobhan Killingbeck, Nicolas Paris, Florent Gimbert, Jonathan Hawkins, Samuel Doyle, Neil Ross, Matthew Peacey, Stephen Livingstone, Ryan Ing, Remy Veness, Lisa Craw, Sian Thorpe, Andrew Sole, Angus Moffatt, and Bernd Kulessa and the Additional members of the SLIDE Project team

Through August-September 2015, a surface depression  was observed in ArcticDEM data near the south lateral margin of Isunnguata Sermia (IS), 0.88 km2 in area and with 30 m maximum deflection. This ‘surface anomaly’, alongside flooding and sediment deposition in the IS foreland, was interpreted as the surface expression of a draining subglacial lake, with subsequent multi-year recovery of the surface elevation occurring as the lake recharged was inferred. Geophysical surveys were conducted through 2023-2025 to investigate lake dynamics over and around the surface anomaly. Reported here is the combined interpretation of active- and passive-source seismic analyses, aiming to image basal topography and determine the presence of a recharged subglacial lake.  

The active-source array comprised 48 vertical-component geophones installed in a 2D profile, recording seismic energy made at a surface impact source; the passive acquisition included a dense grid of Fairfield 3-component seismic nodes, buried in a shallow augur-hole to optimise coupling. By combining active- and passive-source seismic reflectivities, amplitude-versus-angle (AVA) curves can be populated across 0-50° angle range, thus allowing the material properties either side of the glacier bed to be characterised.  Subglacial water, either as a deep lake body or in saturated sediment, would produce negative-polarity reflectivity, given the acoustic softness of water versus the overlying ice. 

Rather than the planar and specular reflectivity often associated with subglacial lakes, seismic profiles show a sloping and rugose bed. Seismic reflection polarities suggest hard basal conditions. AVA analysis, extending from near-zero incidence to the ~50° critical angle, shows consistent positive polarities across all identified bed reflections, suggesting a substrate that is acoustically harder than the overlying ice – for example, consolidated sediment or bedrock. This insight is supported with constraint from passive seismic analysis of seismic velocities beneath the ice, something not typically possible with active-source data alone. These AVA responses are observed inside and outside of the surface anomaly.  Seismic analysis therefore suggests no evidence of significant water saturation or, indeed, a lake beneath the glacier bed. However, with vertical resolution no better than ~10-15 m, we cannot exclude the possibility of water films or small sediment pockets immediately beneath the glacier bed. 

We conclude that any water feature previously inferred from ArcticDEM data was not present during seismic surveying and is therefore transient. Beyond IS, this work questions the degree to which examples in the wider archive of active subglacial lakes may be similarly transient, and expands the range of subglacial settings in which water can accumulate. 

How to cite: Booth, A., Killingbeck, S., Paris, N., Gimbert, F., Hawkins, J., Doyle, S., Ross, N., Peacey, M., Livingstone, S., Ing, R., Veness, R., Craw, L., Thorpe, S., Sole, A., Moffatt, A., and Kulessa, B. and the Additional members of the SLIDE Project team: Seismic observations reveal a hard-bedded drained subglacial lake basin beneath Isunnguata Sermia, West Greenland , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1960, https://doi.org/10.5194/egusphere-egu26-1960, 2026.

EGU26-2281 | Orals | CR2.3

Patchy subglacial drainage systems: observations and modelling 

Christian Schoof and Gabriela Racz

Subglacial water pressure time series from instrumented boreholes provide widespread evidence for the formation of hydraulically disconnected regions at the bed. These do not exhibit the typical diurnal pressure oscillations that indicate a connection to the melting glacier surface during summer. Importantly, the spatial extent of hydraulic disconnection can evolve over time. This is a feature of borehole data sets from both, sub-Arctic glaciers where a cold surface layer quickly seals water-filled boreholes from the surface through freezing, and from temperate mid-latitude glaciers. Current two-dimensional subglacial drainage models do not allow for the connectivity of the drainage system to evolvein time, and in fact, do not allow for the complete shut-down of the system anywahere. In this presentation, we review the observational evidence, focusing on a data set obtained at a small polythermal valley glacier in the southern Yukon Territory, Canada. We document the rapid switching of sizeable (~ 1 ice thickness in extent) parts of the bed from disconnected to connected and back again, driven by the resumption of surface melt resumes following periods of summer snow cover. We show how current drainage models need to be modified to account for suc switching behaviour, and discuss the wider implications of these modifications on drainage system behaviour and glacier dynamics. In particular, we show that switching behaviour can explain the typically observed high water pressures under glaciers during winter, and how this creates conflict with widely used friction laws. We also show how hydraulic switching may limit the ability to pump water out of the bed, which has been suggested elsewhere as a technically plausible mechanism for artificially slowing glacier flow.

How to cite: Schoof, C. and Racz, G.: Patchy subglacial drainage systems: observations and modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2281, https://doi.org/10.5194/egusphere-egu26-2281, 2026.

EGU26-3041 | ECS | Posters on site | CR2.3

Water/Falls: Coupling stochastic calving and subglacial hydrology at Sermeq Kujalleq (Store Glacier) 

Samuel Cook, Doug Benn, and Iain Wheel

Calving glaciers (lake-terminating or tidewater) represent a key uncertainty in future glacier projections, particularly for the ice sheets, where they are responsible, respectively, for around 40% of ice mass loss (Greenland), and nearly 100% (Antarctica). Accurately modelling these glaciers into the future is therefore crucial for being able to forecast future mass loss and the associated sea-level rise. Yet, long-term predictions of the evolution of these systems remain extremely challenging, as both calving and subglacial hydrology, to which these glaciers are highly sensitive, are difficult and/or expensive to model at longer timescales.

One possible solution to better model long-term calving is to represent it as a stochastic process based on the theory of self-organised criticality. Calving can be typified by two types of self-organisation around, respectively, ice cliffs (serac-style events) and ice tongues (full-thickness events). We show that both modes of calving can be influenced by subglacial hydrology.

Here, we therefore present recent work building on the calving implementation of the stochastic crevasse-depth calving function in the open-source ice-flow model, Elmer/Ice, allowing significant improvements in long-term predictions of calving rates and styles. We couple the new calving implementation with the version of the Glacier Drainage System (GlaDS) subglacial hydrology model available in the Elmer/Ice code and present results from a Greenlandic tidewater glacier, Sermeq Kujalleq (Store Glacier). This allows us to explore the interaction of calving, subglacial hydrology, and meltwater plumes, and also provides useful insight for similar future modelling efforts. Using the capabilities of the Elmer/Ice model to resolve the full 3D stress field and allow unconstrained terminus geometries gives us unparalleled insight into the melt-driven serac calving that results from undercutting of the terminus. Furthermore, the subglacial hydrology modelled by GlaDS can directly influence full-thickness calving through increased basal water pressure promoting fractures near the base of the glacier. Consequently, we show that coupled hydrology-calving modelling promotes increased calving in summer when water pressures are high compared to winter.

How to cite: Cook, S., Benn, D., and Wheel, I.: Water/Falls: Coupling stochastic calving and subglacial hydrology at Sermeq Kujalleq (Store Glacier), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3041, https://doi.org/10.5194/egusphere-egu26-3041, 2026.

EGU26-3544 | ECS | Posters on site | CR2.3

Modelling the Geomorphology and Hydrology of Supraglacial Meltwater Channels 

Gianluca Bianchi, Sammie Buzzard, Jonathan Hawkins, and Mike Prior-Jones

Supraglacial channels are a primary pathway for transporting surface meltwater across ice sheets and ice shelves, and their geomorphology plays a key role in controlling meltwater routing. Meltwater commonly drains into supra- and subglacial features, where it can influence ice dynamics and mass loss. As surface melt rates increase under a warming climate, accurately constraining meltwater inputs to these systems becomes increasingly important.

While previous studies have modelled supraglacial channel evolution, few have explicitly accounted for the effects of solar radiation and spatially variable shear stresses on channel geometry. Here, we present a numerical model that simulates the temporal evolution of a supraglacial channel cross-section, incorporating atmospheric and radiative forcing, as well as hydraulic processes. Sensitivity analyses reveal that water temperature is a dominant control on channel incision, even for small variations in temperature. Additional simulations explore how water temperature evolves along the length of a channel and its implications for melt-driven erosion.

By explicitly resolving water temperature and energy exchange, this work provides a more complete description of supraglacial channel geomorphology. These results can be combined with field observations to improve estimates of meltwater routing and drainage volumes, with implications for surface hydrology modelling and ice-sheet mass-loss projections.

 

How to cite: Bianchi, G., Buzzard, S., Hawkins, J., and Prior-Jones, M.: Modelling the Geomorphology and Hydrology of Supraglacial Meltwater Channels, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3544, https://doi.org/10.5194/egusphere-egu26-3544, 2026.

Moulins serve as critical hydrological conduits on the Greenland Ice Sheet (GrIS), facilitating the transfer of surface meltwater to the subglacial bed and directly modulating basal lubrication and ice velocity. Despite their significance, automated detection remains difficult; moulins are often sub-pixel scale in standard satellite imagery and are frequently misidentified as crevasses or inactive stream segments due to spectral overlap. This study introduces GrIS-MDM (GrIS Moulin Detection Model), a novel hydrology-informed framework designed to automate moulin extraction using ultra-high-resolution (0.06 m) unmanned aerial vehicle (UAV) imagery.

The GrIS-MDM framework synergises topographic data from Digital Elevation Models (DEMs) with spectral information from Digital Orthophotography Maps (DOMs) through a sequential tripartite workflow. The process begins by identifying tubular depressions using a contour-derived K-index to effectively eliminate shallow noise and surface artifacts. Subsequently, a multistage attention ResU-Net (MAResU-Net) is implemented to segment supraglacial river networks, utilising an automated sample collection protocol that substantially reduces manual labelling requirements. Finally, topological constraints are applied to isolate true moulins at river termini, distinguishing them from spurious depressions within the river interiors.

Validation conducted in the Sermeq Avannarleq region yielded a recall of 0.795 and a precision of 0.729. Experimental results demonstrate that GrIS-MDM achieves a 20.4% improvement in F1-score over traditional depth-based sink-filling methods. Integrating these detected moulins into hydrological models increased the spatial consistency of reconstructed stream networks by 5.8%. Furthermore, drainage analysis confirmed the model’s accuracy, with simulated water capture (90.8%) closely aligning with ground-truth observations (92.3%). Sensitivity tests indicate the framework remains effective at 2-m resolution, suggesting strong potential for deployment with high-resolution satellite platforms such as WorldView or ArcticDEM. This research offers a robust tool for enhancing high-precision supraglacial hydrological modelling and refining GrIS mass balance assessments.

How to cite: Chen, P., Chen, R., Cheng, X., and Chen, Z.: GrIS-MDM: A Hydrology Knowledge-Based Framework Combining Deep Learning Network for Moulin Detection Using Ultrahigh-Resolution UAV Imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4728, https://doi.org/10.5194/egusphere-egu26-4728, 2026.

EGU26-5028 | ECS | Orals | CR2.3

Thermal characteristics of Greenlandic ice-marginal lakes derived from in-situ temperature data 

Peter Tuckett, Connie Harpur, Alex Scoffield, Duncan Quincey, Hannah Barnett, Joshua Abrahams, Joseph Mallalieu, Lauren Rawlins, Jenna Sutherland, Christopher Merchant, R. Iestyn Woolway, Laura Carrea, Niall McCarroll, Weijia Wang, and David Rippin

Large parts of the Greenland Ice Sheet are fringed by ice-marginal (or ice-contact) lakes. These lakes have increased in number and size as a result of enhanced ice melt and the retreat of the ice sheet margin over recent decades. It has historically been assumed that Greenlandic ice-marginal lakes exist at a relatively uniform temperature of around 1°C year-round, thus having minimal influence on ice dynamics and subaqueous melt rates at the ice-water interface. However, there are almost no in-situ temperature measurements to test this hypothesis, meaning their influence on future ice sheet behaviour remains unclear. Here, we present continuous time series of lake water temperatures collected between July 2024 and August 2025, within three lakes on the western margin of the Greenland Ice Sheet. The results show that lake surface temperatures reached highs exceeding 10°C, with water temperatures above 4°C throughout the entire water column of one study lake during summer months. Summer stratification often persisted for several weeks, whilst inverse stratification was observed when water temperatures fell below 4°C. During winter months, surface ice cover maintained stable inverse stratifications, with lake temperatures ranging between 0 and 4 °C. Although lake temperatures remained largely stable during winter, one lake exhibited a cooling trend and significantly higher variability, potentially indicative of continued subglacial meltwater input.

We combine our sub-hourly lake temperature measurements with meteorological, lake turbidity and ice front calving data, enabling us to investigate sub-diurnal to seasonal controls on lake temperature variability. These analyses show how neighbouring lakes can have markedly differing thermal characteristics, likely due to differences in size, localised topography and variable subglacial and supraglacial meltwater inputs. Our results highlight how uniformly cold temperature values are likely unsuitable when modelling ice-lake dynamics, and that lake terminating sectors of the ice sheet may be experiencing greater rates of frontal ablation than previously realised.

How to cite: Tuckett, P., Harpur, C., Scoffield, A., Quincey, D., Barnett, H., Abrahams, J., Mallalieu, J., Rawlins, L., Sutherland, J., Merchant, C., Woolway, R. I., Carrea, L., McCarroll, N., Wang, W., and Rippin, D.: Thermal characteristics of Greenlandic ice-marginal lakes derived from in-situ temperature data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5028, https://doi.org/10.5194/egusphere-egu26-5028, 2026.

Surface melt is a key control on ice sheet mass balance through meltwater runoff, and the surface-to-bed meltwater connection disturbs ice dynamics. The presence of supraglacial lakes (SGLs), a crucial component of the hydrological system, reduces the surface albedo, resulting in heightened solar radiation absorption and consequently enhancing mass loss. However, it is difficult to quantify lake-albedo feedback because little is known about the bottom ablation process, which is difficult to observe and is currently not incorporated in the regional climate models. This research mainly focuses on the simulation of SGL based on the improved GlacierLake_v2 model. Firstly, the specific albedo-depth parameterization for SGL is developed in the western Greenland ice sheet based on satellite observations, and a meteorologically driven runoff module to calculate meltwater input is also incorporated in GlacierLake_v2. Secondly, the SGL-albedo feedback (the melt rate difference between SGL and bare ice) is quantified in Lake BlueSnow, and its influencing factors are explored.

The lake albedo is calculated using narrow-to-broadband conversion, and the lake depth is extracted from ICESat-2. The albedo-depth parameterization is described by an exponential function. Compared to the measured bottom ablation, the GlacierLake_v2 achieves superior performance over the original GlacierLake model, with RMSE reduced by more than 50%. The SGL-albedo feedback exhibits an exponential decline as lake depth increases. Summer snowfall rapidly suppresses the ice sheet surface melt rate while exerting little influence on the lake bottom melting, thereby triggering strong SGL albedo feedback. We are currently developing a distributed SGL model aimed at simulating lake evolution in both horizontal and vertical dimensions and at the volume estimation of buried lakes. There is also the prospect of integrating GlacierLake_v2 into the more comprehensive hydrological model to decrease the uncertainty in surface mass loss predictions.

How to cite: Wu, J., Zheng, L., and Hui, F.: Greenland supraglacial lakes albedo-depth parameterization from multi-source remote sensing: an application of lake-albedo feedback modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5158, https://doi.org/10.5194/egusphere-egu26-5158, 2026.

EGU26-5264 | Orals | CR2.3

Integrating Microwave Remote Sensing with Physical Models to Reveal Melt Dynamics and Structural Variability in Queen Maud Land 

Andreas Colliander, Nicole-Jeanne Schlegel, Alamgir Hossan, Catherine Walker, Joel Harper, Juha Lemmetyinen, and Aku Riihelä

The Queen Maud Land (QML) sector of East Antarctica comprises a complex system of grounded ice sheet and fringing ice shelves that regulate ice discharge to the Southern Ocean. Ice-sheet evolution in this region is controlled by interactions between atmospheric forcing, katabatic winds, and bedrock topography, producing strong spatial variability in accumulation, flow, and thermal regimes. While the bordering ice shelves currently act as stabilising buttresses, they are sensitive to oceanic heat intrusions, changing sea-ice conditions, and episodic surface melt. Melt–refreeze processes enhance firn compaction, weaken surface integrity, and may precondition ice shelves for hydrofracture under future warming, despite QML presently exhibiting a positive mass balance trend.

We investigate the thermal and structural evolution of snow, firn, and ice in QML using an integrated framework that combines multi-frequency passive microwave observations with physically based modelling. Passive microwave measurements provide complementary sensitivity to near-surface melt processes and deeper firn and ice structure, enabling the detection of both contemporary melt signals and long-term subsurface changes. Lower-frequency observations penetrate deep into the firn and ice column, whereas higher-frequency observations respond to surface temperature, liquid water content, and accumulation variability.

Snow, firn, and ice evolution is simulated using the Glacier Energy and Mass Balance (GEMB) model, running on the Ice Sheet and Sea Level System Model (ISSM), providing vertical profiles of temperature, density, and liquid water content driven by meteorological forcing. These profiles are used to forward-model microwave brightness temperatures with the Microwave Emission Model of Layered Snowpacks (MEMLS) across frequencies from 1.4 to 36.5 GHz, accounting for densification and refrozen ice layers. Modelled brightness temperatures are evaluated against satellite observations, providing twice-daily coverage of QML since 2010.

We present spatial and temporal patterns of grounded ice-sheet structure, surface and subsurface temperature variability, fresh snow accumulation, and ice shelf melt signatures, together with residuals between observed and modelled brightness temperatures. Our results demonstrate the value of radiometric modelling for constraining firn structure, melt processes, and ice-shelf vulnerability in regions with sparse in situ data. By integrating passive microwave observations with physical firn models, this work supports improved calibration, initialisation, and confidence in projections of mass balance and structural evolution in the Queen Maud Land sector of East Antarctica.

How to cite: Colliander, A., Schlegel, N.-J., Hossan, A., Walker, C., Harper, J., Lemmetyinen, J., and Riihelä, A.: Integrating Microwave Remote Sensing with Physical Models to Reveal Melt Dynamics and Structural Variability in Queen Maud Land, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5264, https://doi.org/10.5194/egusphere-egu26-5264, 2026.

EGU26-5266 | Posters on site | CR2.3

Interseasonal persistence of large subglacial channel on Hintereisferner, Austria. 

Céline Walker, Nikola Jovanovic, and Samuel Cook

Understanding the subglacial hydrology of glaciers is key in adequately modelling ice flow and future retreat of glaciers under climate change. Subglacial drainage systems are observed and modelled to change with the seasons, varying between an inefficient, distributed drainage system in winter and an efficient, channelised drainage system during the melt season. This directly influences a glacier’s basal flow velocity. Subglacial channels close at the end of the melt season by ice creep and the decrease of melt reducing subglacial discharge, and are typically supposed to disappear completely on many Alpine glaciers before the start of the next melt season. We modelled the evolution of the subglacial discharge system over the course of a year on Hintereisferner, Austrian Alps, using the Glacier Drainage System model (GlaDS). Additionally, we did three ground-penetrating radar (GPR) acquisitions of the glacier tongue over the course of a year (April 2025-March 2026). In both winter and summer acquisitions, en- and subglacial channels could be observed. Besides minor changes in the drainage system, a large subglacial channel was repeatedly detected, indicating possible long-term persistence of channelised drainage throughout the winter despite the expected shutdown of the efficient subglacial drainage system. We present our observations and compare them to the model results. Furthermore, the implications for ice flow and glacier evolution are discussed.

How to cite: Walker, C., Jovanovic, N., and Cook, S.: Interseasonal persistence of large subglacial channel on Hintereisferner, Austria., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5266, https://doi.org/10.5194/egusphere-egu26-5266, 2026.

EGU26-5730 | ECS | Orals | CR2.3 | Highlight

Understanding supraglacial drainage networks on mountain glaciers using high‑resolution orthophotos, UAV imagery and field data 

Holly Wytiahlowsky, Chris Stokes, Rebecca Hodge, and Caroline Clason

Supraglacial channels play a fundamental role in efficiently transporting surface meltwater across, into, and beyond glacier systems, with implications for surface mass balance, glacier dynamics, and the hydrochemistry of glacier runoff. Although such channels have been frequently documented in ice sheet settings, the resolution of satellite imagery makes similar studies on mountain glaciers challenging, and field observations remain scarce. Here, we combine uncrewed aerial vehicle (UAV) imagery, field measurements, and historical aerial photographs to conduct high-resolution mapping of supraglacial channels on Glacier du Brenay in the Swiss Alps, which provides new insights into their distribution and characteristics. Our results reveal a dense pattern of broadly dendritic channel networks influenced by ice surface structures. We find that most first-order channels, which are only visible in UAV imagery, terminate englacially in crevasses. Consequently, englacial routing is likely more widespread at Glacier du Brenay than suggested by coarser resolution imagery, where the larger and more detectable channels often flow off the glacier terminus. Channel size and distribution are influenced by the glacier’s surface profile, which dictates the location and extent of channel catchments. Larger upstream-originating catchments are associated with increased channel dimensions, and where deeply incised channels from these catchments flow off the terminus, they are associated with rapid retreat at the proglacial margin. We find that continuous debris cover produces shallow channels and results in increased channel roughness, decreased water velocity, and reduced surface lowering rates. In contrast, discontinuous debris is associated with the highest rates of surface lowering and can produce pitted topography, which also increases channel roughness. Future research should therefore consider small-scale hydrological processes. 

How to cite: Wytiahlowsky, H., Stokes, C., Hodge, R., and Clason, C.: Understanding supraglacial drainage networks on mountain glaciers using high‑resolution orthophotos, UAV imagery and field data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5730, https://doi.org/10.5194/egusphere-egu26-5730, 2026.

EGU26-5759 | ECS | Orals | CR2.3

Modeling interaction between supraglacial melt lakes and calving in transient Antarctic simulations 

Danielle Grau, Mattia Poinelli, Nicole Schlegel, and Alexander A Robel

Supraglacial melt lakes have been linked to large-scale Antarctic ice shelf collapse, such as those observed at Larsen A and B ice shelves in the early 2000s. As Earth’s climate warms, surface melt and the formation of supraglacial melt lakes are expected to increase. Currently, there is no representation of the impacts of supraglacial melt lakes in large-scale ice sheet modeling. In this work, we implement physics-based parameterizations of supraglacial melt lakes in the Ice Sheet and Sea-Level System Model (ISSM) to simulate their effect on fracture propagation and calving. We described a new physics-based modeling protocol for capturing realistic interactions between surface melt and calving. We show the influence of including these interactions on benchmark ISMIP6 simulations by comparing them to simulations which either (a) do not simulate supraglacial melt lakes or (b) simulate instantaneous collapse of all floating ice in Antarctica. We further discuss caveats with this approach and directions for future research.

How to cite: Grau, D., Poinelli, M., Schlegel, N., and Robel, A. A.: Modeling interaction between supraglacial melt lakes and calving in transient Antarctic simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5759, https://doi.org/10.5194/egusphere-egu26-5759, 2026.

Moulins are vertical conduits on the Greenland ice sheet (GrIS) formed by hydrofracturing of crevasses and supraglacial lakes. They determine where, when, and how much surface meltwater can be drained to ice sheet bed, thereby controlling subglacial water pressure, developing subglacial drainage system, and eventually affecting ice motion. Therefore, obtaining moulin distribution over extended time period is essential for understanding variability in surface-to-bed meltwater connections. Using 10 m Sentinel-2 satellite imagery, we map interannual moulin distributions on the southwest GrIS during late summer from 2016 to 2021, as well as the seasonal moulin evolution throughout the warm 2019 summer. We find that widespread moulins drain the majority of meltwater into the ice sheet during 2016-2021. They are even denser in warmer years with larger proportions of meltwater drainage. Notably, a considerable number of moulins recur in multiple years and act as stable meltwater connections. During the warm 2019 summer, moulins first increase substantially at low elevations in June, then expand to high elevations in July, and remain relatively stable in August. As a result, surface-to-bed meltwater connections are spatially localized early in the melt season and become more discrete as the melt season progresses.

How to cite: Wang, Y. and Yang, K.: Satellite mapping of the varying moulin distribution on the southwest Greenland ice sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6241, https://doi.org/10.5194/egusphere-egu26-6241, 2026.

Meltwater buffering in the firn of glaciers, ice caps and ice sheets is an important, yet relatively uncertain, process that determines their mass balance. In the firn layer, meltwater and rain percolate downwards until it is buffered in wet layers, refrozen, or runs off. The efficiency of water retention determines the ratio of refreezing to runoff, while the vertical distribution of refreezing has a long-lasting impact on the subsurface density, heat conductivity and temperature profile. An accurate representation of water buffering is particularly crucial for estimating future runoff from the Greenland Ice Sheet. There, the formation of ice lenses in the former percolation zone could dramatically reduce the buffering capacity of the firn layer. Current firn models either are empirically-based and struggle to represent the complex processes determining water buffering or are physics-based but computationally expensive due to strong non-linearities in the governing equations.

Here, we present the intermediate-complexity percolation model FirnPerc that aims to capture the relevant water processes in firn within a fast and stable computational framework. Matrix percolation through firn is represented as gravity-driven flow, neglecting capillary forces. In cases of low water content and water flux, model layers can be partially wetted and can therefore remain below the melting point on average for a while. When water flow stalls on ice lenses, the model can form a slush layer. Gradual water percolation through ice lenses is parameterised, with exponentially decreasing efficiency for increasing ice layer thickness. Finally, in the absence of an explicit horizontal flow description, slush water is assumed to run off very slowly. With these process parameterizations, FirnPerc can resemble important features of Greenlandic firn, such as fast, deep percolation at the start of the melting season, ice lenses with slush layers on top, and deep, water-rich year-round aquifers.

How to cite: van de Berg, W. J.: FirnPerc: An intermediate-complexity water percolation model for firn, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7173, https://doi.org/10.5194/egusphere-egu26-7173, 2026.

EGU26-7285 | ECS | Posters on site | CR2.3

Optimising detection of Greenland's active subglacial lakes with DEMs: evaluating coregistration and detrending strategies 

Diego Moral Pombo, Malcolm McMillan, Jade Bowling, Dominic Hardy, Romilly Close, and Joseph Phillips

The GLOBE (Greenland Subglacial Lake Observatory) project aims to create a comprehensive inventory of Greenland's active subglacial lakes through systematic analysis of high-resolution Digital Elevation Models (DEMs) combined with satellite altimetry data. In particular, the complete 2-meter resolution ArcticDEM database covering the entire ice sheet between 2008 and 2025 is utilised for this purpose. Since initial proof-of-concept studies demonstrated the viability of detecting subglacial lake dynamics using elevation variance, substantial progress has been made in extending this approach across larger spatial scales and more diverse glaciological conditions.

In this work, we present methodological refinements necessary for robust, systematic detection of subglacial lake signatures at the ice-sheet scale. We evaluate the impact of different coregistration methods (including no coregistration) on the reliability of the standard deviation of elevation maps used for lake identification. Additionally, we assess the effectiveness of detrending long-term ice-sheet elevation changes to isolate the shorter-term, localised elevation variations associated with subglacial lake drainage and filling events. As the project scales to cover all the ice sheet, understanding how these processing choices affect detection accuracy, precision, and the separation of signal from noise is critical for ensuring robust, reproducible results.

Preliminary results presented here offer insights into the relative importance of the different parameters and steps involved in the GLOBE pipeline and their contribution to lake identification. We demonstrate how these results inform best practices for systematic subglacial lake mapping across Greenland and the subsequent integration of subglacial hydrology into larger-scale ice sheet models, thereby improving predictions of ice sheet stability and mass loss.

How to cite: Moral Pombo, D., McMillan, M., Bowling, J., Hardy, D., Close, R., and Phillips, J.: Optimising detection of Greenland's active subglacial lakes with DEMs: evaluating coregistration and detrending strategies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7285, https://doi.org/10.5194/egusphere-egu26-7285, 2026.

EGU26-7976 | ECS | Orals | CR2.3

Subglacial lake drainage event impacts basal hydrology and dynamics of Greenland outlet glacier 

Armin Dachauer, Andrea Kneib-Walter, Ethan Welty, and Andreas Vieli

Subglacial lakes are important hydrological reservoirs within the Greenland Ice Sheet, primarily fed by meltwater from the surface that reaches the bed. Episodically, these lakes drain, releasing vast volumes of water into the subglacial drainage system and thereby altering basal hydrology and local ice dynamics. A warming climate is expected to intensify surface meltwater production and potentially increase the frequency of subglacial lake drainage events. However, direct observations of such events remain scarce, limiting our understanding of their driving mechanisms and impacts on the subglacial system.

 

Here we document a subglacial lake at Eqalorutsit Kangilliit Sermiat, a major tidewater outlet glacier in Southwest Greenland. This subglacial lake typically drains once or twice per melt season. We observed one such event using time-lapse imagery, GNSS measurements, terrestrial radar interferometry, and digital elevation models (DEMs). From these observations, we estimate a drainage volume of approximately 0.3 km3, and local ice surface lowering that exceeds 50 m. Additionally, we delineated the lake outline and were able to estimate lake drainage rates and refilling rates. Our results further indicate a (partial) re-routing of the subglacial drainage system following the lake drainage event. As the lake drained, we observed an acceleration of the glacier’s terminus region and the emergence of a large sediment-rich plume. This highlights the profound influence of episodic subglacial lake drainage on glacier dynamics as well as fjord circulation and ecosystems.

How to cite: Dachauer, A., Kneib-Walter, A., Welty, E., and Vieli, A.: Subglacial lake drainage event impacts basal hydrology and dynamics of Greenland outlet glacier, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7976, https://doi.org/10.5194/egusphere-egu26-7976, 2026.

EGU26-8117 | ECS | Orals | CR2.3

Distributed, Multi-Physical Fibre Optic Sensing of the Isunnguata Sermia Englacial Hydraulic System and its Impact on Glacial Dynamics 

Lucas Fabbri, Florent Gimbert, Nicolas Paris, Thomas Chauve, Alexandre Michel, Tifenn Le Bris, Luc Picard, Romain Duphil, Firmin Fontaine, Guilhem Freche, Samuel H. Doyle, Sian Thorpe, Stephen J. Livingstone, and Andrew Sole

The transfer of surface meltwater to the base of the Greenland Ice Sheet modulates basal sliding, which controls ice loss into the ocean. The way in which water reaches the glacier bed, organizes itself near the ice-bed interface, and affects ice dynamics remains poorly understood due to limited observations. In this study, we present and interpret a multi-physical observational dataset from Isungnuata Sermia, West Greenland, acquired during the 2024 and 2025 melt seasons as part of the REASSESS and SLIDE projects.

We show how Distributed Fibre Optic Sensing (DFOS) measurements combined with meteorological observations and models, and Global Navigation Satellite System (GNSS) measurements of surface ice motion, provide observational constraints on and improve our conceptual understanding of the surface-to-bed hydrological connection. We deployed fibre optic cables at the surface and in four 600 m boreholes, providing measurements of temperature, strain, and seismicity at thousands of sensing points at the surface, and through the full depth of the glacier.

We observe that seismic activity is temporally linked with surface melt on a daily and weekly scale and evolves over time in alignment with the coalescence of surface channels. We apply Matched-Field Processing (MFP) beamforming to detect and locate seismic sources, aiming to resolve the vertical extent of fracturing related to water input. We observe the migration of some high-frequency seismic events to greater depths during periods of high runoff. This process is coincident with ice surface acceleration and subsequent deceleration events. Temperature and strain measurements from the DFOS system indicate highly variable distributions of temperature and deformation, which enable exploration of the prevalence and importance of englacial fracturing in surface-to-bed water transport.

Together, these data offer potential insights into the mechanism of fracture-driven water transport, basal pressure increase, and subsequent regulation and dissipation via subglacial-water-channel development, and the relationship of these processes to glacial dynamics.

How to cite: Fabbri, L., Gimbert, F., Paris, N., Chauve, T., Michel, A., Le Bris, T., Picard, L., Duphil, R., Fontaine, F., Freche, G., Doyle, S. H., Thorpe, S., Livingstone, S. J., and Sole, A.: Distributed, Multi-Physical Fibre Optic Sensing of the Isunnguata Sermia Englacial Hydraulic System and its Impact on Glacial Dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8117, https://doi.org/10.5194/egusphere-egu26-8117, 2026.

EGU26-8700 | Orals | CR2.3

Frictional Melt–Sustained Subglacial Hydrology Modulates Ice–Bed Coupling at an Antarctic Peninsula Outlet Glacier 

Yuting Dong, Ji Zhao, Michael Wolovick, Veit Helm, Steven Franke, Jan Wuite, Lukas Krieger, Dana Floricioiu, Thomas Kleiner, Daniela Jansen, Lea-Sophie Höyns, Martin Rückamp, and Yanfei Zhong

Seasonal acceleration of Antarctic Peninsula outlet glaciers is commonly attributed to surface melt–driven basal lubrication and ocean forcing. However, the role of internally generated basal meltwater, independent of seasonal surface inputs, remains poorly constrained by observations, despite its potential to introduce year-round dynamic sensitivity that is not captured by seasonally forced frameworks. Here we investigate how non-seasonal subglacial hydrology influences the dynamics of Fleming Glacier, a rapidly evolving outlet glacier draining into Wordie Bay on the western Antarctic Peninsula.

Using time-resolved digital elevation models (2011–2024) together with satellite-derived surface velocity and basal drag estimates, we identify an actively evolving subglacial water reservoir beneath the fast-flowing lower trunk of the glacier. Episodic filling and drainage of this reservoir produce multi-meter surface height anomalies that are temporally coincident with changes in ice velocity and basal drag. These signals occur predominantly during austral winter and exhibit weak or absent annual periodicity, indicating that they are not driven by seasonally varying surface meltwater input.

Energy-budget considerations and spatial patterns of hydraulic potential suggest that the reservoir is sustained primarily by internally generated basal meltwater produced through frictional heating, rather than by surface or oceanic meltwater sources. Episodic drainage events transiently reduce effective pressure at the ice–bed interface, promoting short-lived acceleration and spatial reorganization of basal drag upstream of the grounding line.

Our results demonstrate that internally driven, non-seasonal subglacial hydrology can modulate ice–bed coupling on multi-year timescales, highlighting an additional mechanism of outlet glacier variability that operates independently of seasonal climate forcing.

How to cite: Dong, Y., Zhao, J., Wolovick, M., Helm, V., Franke, S., Wuite, J., Krieger, L., Floricioiu, D., Kleiner, T., Jansen, D., Höyns, L.-S., Rückamp, M., and Zhong, Y.: Frictional Melt–Sustained Subglacial Hydrology Modulates Ice–Bed Coupling at an Antarctic Peninsula Outlet Glacier, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8700, https://doi.org/10.5194/egusphere-egu26-8700, 2026.

EGU26-8915 | Posters on site | CR2.3

Temporary slow-down associated with drainage of a large subglacial lake, Totten Glacier, East Antarctica 

J. Paul Winberry, Chad Greene, Felicity McCormack, Sue Cook, and Christine Dow

We present observations documenting the drain–fill cycle of a large subglacial lake and the associated velocity response on the Totten Glacier, East Antarctica. The lake transitioned from a period of stability to rapid drawdown, dropping by more than 50 m in less than a year. Following drainage, glacier flow speed decelerated by ~100 m yr⁻¹ (~20%) over the lake and by ~30 m yr⁻¹ in a region immediately downstream. We hypothesize that the pronounced slowdown over the lake reflects complete drainage and increased basal traction associated with grounding, while the downstream deceleration results from disruption of the subglacial hydrologic system. Over the subsequent three years, as the lake refilled, glacier flow speeds recovered to pre-drainage levels.

 

How to cite: Winberry, J. P., Greene, C., McCormack, F., Cook, S., and Dow, C.: Temporary slow-down associated with drainage of a large subglacial lake, Totten Glacier, East Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8915, https://doi.org/10.5194/egusphere-egu26-8915, 2026.

EGU26-9501 | ECS | Posters on site | CR2.3

Emulating a Subglacial Hydrology Model with a Neural Operator 

Nikola Jovanovic, Samuel Cook, Thomas Zwinger, Johannes Fürst, and Céline Walker

Subglacial hydrology exerts an important control on ice flow and influences the evolution of downstream hydrology, as well as the occurrence of glacial lake outburst floods. However, large-scale modelling of subglacial hydrology remains computationally expensive due to the presence of nonlinear processes.

Within our DeLIGHT (Deep-Learning-Informed Glacio-Hydrological Threat) framework, we aim at enabling coupled simulations of ice flow, subglacial hydrology, and downstream hydrology, with the goal of improving predictions of ice flow evolution and the timing of peak runoff. For this purpose, we will leverage recent advances in deep learning. As a first step, this research focuses on the development of a subglacial hydrology emulator trained using output from the Glacier Drainage System (GlaDS) model implemented within Elmer/Ice, with the aim of applicability to mountain glacier catchments worldwide. The emulator is based on a class of deep learning architecture called neural operators, which allow for better generalisation compared to classical neural networks.

To generate the training set, GlaDS is forced using meltwater inputs derived from a calibrated degree-day model, which is driven by daily climate data spanning the 2000–2010 period. We select 70 glaciers spanning a wide range of physiographic characteristics across Svalbard, Scandinavia, the Alps, and Central and Southeast Asia to provide a representative range of mountain-glacier subglacial hydrological scenarios within the training set. We present results from the training simulations and initial directions for the development of the emulator.

How to cite: Jovanovic, N., Cook, S., Zwinger, T., Fürst, J., and Walker, C.: Emulating a Subglacial Hydrology Model with a Neural Operator, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9501, https://doi.org/10.5194/egusphere-egu26-9501, 2026.

Beneath the Antarctic Ice Sheet, active subglacial lakes act as dynamic storage–release nodes that modulate basal water pressure, influence ice flow, and regulate freshwater delivery to grounding zones. However, inventories and time series derived from single sensors remain incomplete due to limited spatial coverage, short mission lifetimes, and cross-sensor inconsistencies in sampling geometry and accuracy. Here we present a continent-wide, multi-mission framework that integrates three decades of satellite altimetry with high-resolution REMA strip DEMs to detect and monitor active subglacial lakes. We harmonize reprocessed ERS-1/2 and Envisat radar altimetry, ICESat and ICESat-2 laser altimetry, and CryoSat-2 swath measurements through local annular co-registration and a crossover-zone representativeness correction, enabling internally consistent, lake-scale elevation change estimates across sensors. The approach resolves subtle elevation variability, refines outlines delineation, and reconstructs multi-decadal (>30 years) filling–drainage histories. Applied to the Byrd Glacier basin, the framework increases the number of confirmed active lakes from 23 in existing inventories to 74, including 51 newly identified systems, and delivers refined outlines and time series for each lake. The resulting records reveal structured lake–lake interactions, motivating a process-based classification of cascading behavior into serial cascades, parallel co-variation, and terminal confluence. Our results indicate that observational incompleteness remains a primary limitation on Antarctic subglacial hydrology, and demonstrate that systematic multi-mission fusion can substantially improve detection, connectivity inference, and quantification of storage–release variability, providing stronger observational constraints for linking basal hydrology to ice dynamics and improving ice-sheet projections.

How to cite: Yang, T., Liang, Q., Li, T., and Cheng, X.: A novel framework for detecting and monitoring Antarctic active subglacial lakes using multi-source remote sensing data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9771, https://doi.org/10.5194/egusphere-egu26-9771, 2026.

EGU26-11462 | Posters on site | CR2.3

Shortwave Penetration Drive Subsurface Warming and Melt on Langhovde Glacier, East Antarctica 

Jun Saito and Masahiro Minowa

Surface meltwater on ice shelves, together with runoff from upstream grounded ice, can pond and drain into crevasses, raising water pressure and promoting hydrofracturing. However, the timing of meltwater storage and release in coastal ablation and blue ice areas remains poorly constrained because continuous subsurface temperature records are scarce. Here we present one year of subsurface ice-temperature measurements from the blue ice area on Langhovde Glacier in coastal East Antarctica from January 2024 to January 2025, revealing persistent internal warming and a vertical temperature structure consistent with absorption of shortwave below the surface. We combine our observations with a coupled surface energy balance and firn model to isolate the effect of shortwave penetration into the surface. Simulations without subsurface shortwave absorption fail to reproduce the observed warming and its seasonal persistence, whereas including shortwave penetration substantially improves the simulated vertical temperature profile and supports an interpretation involving subsurface melt and refreezing. Observed near-surface ice temperature was ~3 °C higher than that model output. At 10 m depth, ice temperature was ~−6 °C, about 4 °C warmer than the site’s mean air temperature. These results indicate that shortwave driven subsurface heat storage is likely a key control on near surface thermal conditions in Antarctic blue ice area and may influence the seasonal opening and closure of meltwater pathways, thereby affecting the timing of runoff discharge to downstream ice shelves.

How to cite: Saito, J. and Minowa, M.: Shortwave Penetration Drive Subsurface Warming and Melt on Langhovde Glacier, East Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11462, https://doi.org/10.5194/egusphere-egu26-11462, 2026.

EGU26-11784 | ECS | Posters on site | CR2.3

Continental-scale mapping of Antarctic supraglacial hydrology using machine learning 

Emily Glen, Amber Leeson, Frank Donachie, Malcolm McMillan, and Joseph Phillips

Surface meltwater influences Antarctic ice-shelf stability by enhancing melt, lowering albedo, and promoting hydrofracture. Although supraglacial hydrology is now recognised as widespread across Antarctica, existing meltwater feature records vary in spatial resolution and temporal sampling. Recent work tends to only classify supraglacial lakes while inconsistently representing more transient features such as slush, underestimating the full extent of surface meltwater. Furthermore, traditional threshold-based supraglacial meltwater mapping approaches require extensive manual post-processing and are difficult to scale; machine learning offers a promising alternative but requires systematic evaluation to ensure classifiers generalise reliably across time and space.

Here, as part of the ESA 5D Antarctica project, we present a new continent-wide, high-resolution record of supraglacial hydrology across all Antarctic ice shelves from 2016 to 2026. The dataset is derived from ~135,100 Sentinel-2 images using supervised machine learning implemented in Google Earth Engine. To systematically evaluate machine-learning approaches, which remain underexplored in glaciological applications and are often applied without rigorous validation, we compared five algorithms: Random Forest, Gradient Boosting Decision Trees, Classification and Regression Trees, Support Vector Machines, and k-Nearest Neighbours. Each was assessed using five complementary validation experiments: repeated cross-validation to assess internal consistency, independent validation against expert-labelled data to test external accuracy, leave-one-year-out cross-validation to evaluate temporal transferability, leave-one-region-out testing to assess spatial transferability, and controlled label corruption to quantify sensitivity to annotation error. Random Forest achieved the most consistent performance and ranked first overall with a mean macro-F1 score of 0.992 and was selected for continent-wide deployment.

The resulting dataset provides monthly classifications of supraglacial hydrology, distinguishing open meltwater features, including lakes, channels, and water-filled crevasses, from non-open meltwater features such as saturated firn and slush. The dataset is delivered alongside an interactive cloud-based application that enables users to visualise, classify, and export products on demand. By resolving Antarctic surface hydrology at unprecedented spatial and temporal scales and enabling on-demand delineation of meltwater features through a publicly available application, this work supports the assessment of processes relevant to ice-shelf stability and provides constraints for climate and ice-sheet modelling. This capability is increasingly important for understanding the role of surface meltwater in Antarctic ice-shelf systems under future warming.

How to cite: Glen, E., Leeson, A., Donachie, F., McMillan, M., and Phillips, J.: Continental-scale mapping of Antarctic supraglacial hydrology using machine learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11784, https://doi.org/10.5194/egusphere-egu26-11784, 2026.

EGU26-12454 | ECS | Posters on site | CR2.3

Parameterising crevasse field drainage into meltwater routing models for the Greenland Ice Sheet 

Thomas Chudley, Chris Stokes, James Lea, Robert Law, Adam Hepburn, and Caroline Clason

Nearly all meltwater produced on the Greenland Ice Sheet surface is routed through the interior of the ice, and the spatial and temporal patterns – as well as the mode of delivery – of discharge to the bed can have significant consequences for processes including ice fracture, rheology, and basal sliding. Existing suggest that a majority of meltwater in Greenland is transferred to the bed via surface crevasse fields, rather than lakes or moulins. However, in contrast to well-observed phenomena such as supraglacial lake drainages, little work has been done to explore how this process should be parameterised in regional-scale models that route meltwater from the surface to the bed. Here, we explore: (i) how well observations of crevasse field filling and drainage support existing parameterisations based upon linear elastic fracture mechanics (LEFM); (ii) what modifications may need to be implemented to better represent crevasse field hydrology, including the choice of proxy for resistive stress (Rxx) and the inclusion of seasonally-varying stress; and (iii) the potential consequences for effective and sliding at the glacier bed, as represented through subglacial hydrological models.

How to cite: Chudley, T., Stokes, C., Lea, J., Law, R., Hepburn, A., and Clason, C.: Parameterising crevasse field drainage into meltwater routing models for the Greenland Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12454, https://doi.org/10.5194/egusphere-egu26-12454, 2026.

EGU26-13687 | ECS | Orals | CR2.3

Continental-scale observations of seawater infiltration in Antarctic ice shelves reveal an overlooked hydrologic system 

Ian McDowell, Riley Culberg, Clara Nordahl, Victoria Villagomez, Theodore Scambos, and Julie Miller

Dynamic hydrologic networks on and within ice shelves are increasingly recognized as critical controls on ice shelf stability and ice sheet mass loss. To date, ice shelf hydrology has been primarily framed in terms of surface-derived meltwater, including supraglacial pond formation, firn infiltration and refreezing, and meltwater aquifer development. Recent firn modeling suggests that a substantial fraction of Antarctic ice shelf firn lies below sea level, providing extensive pore space that is susceptible to seawater intrusion and brine aquifer formation. Despite this potential, seawater infiltration into porous firn has remained largely unexplored beyond a small number of spatially limited observations, many of which were collected decades ago.

Here, we present the first continental-scale observational assessment of seawater-derived aquifers within Antarctic ice shelves. We analyzed ~145,000 km of airborne radar flightlines and identified diagnostic brine signatures along ~4,500 km of profiles spanning more than 30 Antarctic ice shelves, demonstrating that seawater infiltration occurs wherever suitable observations exist. By reconciling radargrams with available digital elevation models and lidar data, we show that the dominant infiltration mechanisms vary regionally: Antarctic Peninsula ice shelves commonly exhibit large infiltration zones in thin or damaged ice, whereas East Antarctic ice shelves are characterized by localized intrusion along rifts and basal crevasses. We further map the depth of the brine water table across these systems, revealing spatial variability in aquifer geometry linked to ice shelf structure and infiltration mechanism. Climate model projections indicate that regions currently hosting brine aquifers are projected to experience larger future increases in surface meltwater inputs than ice shelf regions without detected brine, highlighting the potential for the development of mixed aquifer systems. Our results demonstrate that seawater infiltration represents a widespread and previously underappreciated hydrologic pathway within Antarctic ice shelves and highlight the need to incorporate these systems into emerging frameworks of ice shelf hydrology and stability.

How to cite: McDowell, I., Culberg, R., Nordahl, C., Villagomez, V., Scambos, T., and Miller, J.: Continental-scale observations of seawater infiltration in Antarctic ice shelves reveal an overlooked hydrologic system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13687, https://doi.org/10.5194/egusphere-egu26-13687, 2026.

EGU26-13736 | Posters on site | CR2.3

Retrieving Supraglacial Lake Depths on George VI Ice Shelf using ICESat-2 

Ian Willis, Cheng Cheng, Ciara Metcalfe, Rebecca Dell, and Alison Banwell

Increasing atmospheric warming is enhancing surface melt across Antarctica, leading to the widespread formation of supraglacial lakes (SGLs) on ice shelves. These lakes play a critical role in ice-shelf stability by promoting hydrofracturing, increasing flexural stresses, and potentially triggering ice-shelf collapse, thereby accelerating grounded ice discharge and sea-level rise. Accurate estimation of SGL depth and volume is therefore essential for understanding Antarctic ice dynamics.

To date, most large-scale SGL depth estimates have relied on optical remote sensing and radiative transfer methods (RTMs), which infer lake depth from spectral attenuation in satellite imagery. While effective, RTMs are sensitive to surface conditions, cloud cover, and water optical properties. The launch of ICESat-2 in 2018 provides a complementary approach, as its photon-counting lidar can detect returns from both lake surfaces and beds, enabling direct depth estimation. Several algorithms have been developed to extract SGL depths from ICESat-2 data, but applications remain spatially limited and none have yet focused on the George VI Ice Shelf (GVIIS).

Here, we present the first retrieval of supraglacial lake depths on the northern GVIIS using ICESat-2 ATL03 and ATL06 data. We apply the Watta algorithm (Datta and Wouters, 2021) to derive along-track SGL depth profiles and compare these results with independent depth estimates obtained using an RTM applied to Sentinel-2 and Landsat 8 imagery. This comparison is used to evaluate the strengths and limitations of ICESat-2–based depth retrievals relative to established optical methods.

Our study provides new constraints on supraglacial lake characteristics on the northern GVIIS and demonstrates the value of integrating active and passive remote sensing approaches to improve assessments of meltwater processes that influence Antarctic ice-shelf stability.

How to cite: Willis, I., Cheng, C., Metcalfe, C., Dell, R., and Banwell, A.: Retrieving Supraglacial Lake Depths on George VI Ice Shelf using ICESat-2, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13736, https://doi.org/10.5194/egusphere-egu26-13736, 2026.

EGU26-14926 | ECS | Posters on site | CR2.3

Modelling subglacial responses to future moulin inputs in the Amundsen Sea Embayment 

Anna-Mireilla Hayden, Christine Dow, Tim Hill, Shivani Ehrenfeucht, and Tyler Pelle

At present, there is minimal surface meltwater over Antarctica and Antarctic subglacial drainage systems are isolated from supraglacial water, differentiating them from the surface meltwater-fed hydrological networks of Greenland. However, projected increases in surface melt across grounded regions of the Antarctic Ice Sheet raise the possibility that surface-to-bed hydrological connections may begin to form via moulins, features known in Greenland to drive seasonal ice velocity variability by modulating subglacial water pressure. In Antarctica, additional seasonal water fluxes into the subglacial drainage system could amplify the effects that subglacial channels have on ice dynamics and sub-ice shelf melt rates, which could, in turn, impact grounding line positions and stability and alter the rate of sea level rise. Here, we investigate the response of the Amundsen Sea Embayment (ASE), where rapid, potentially irreversible changes are underway, to new subglacial meltwater forcing from moulin inputs. To accomplish this, we develop a moulin prediction algorithm that uses surface melt projections at 2100 and 2300 from UKESM and strain rates derived from the Ice Sheet and Sea Level Systems Model (ISSM). We then use these moulin locations and discharges as input to the Glacier Drainage System (GlaDS) subglacial hydrology model. We simulate five consecutive melt seasons followed by an extended recovery period to evaluate whether episodic meltwater inputs leave a long-term imprint on the ASE's drainage system. We provide a mosaic of possible trajectories for ASE's subglacial drainage system by varying GlaDS internal parameters and the strain-rate threshold, complemented by an additional set of experiments that use a randomly generated moulin distribution. This approach allows us to better gauge the sensitivity and responsiveness of the ASE's drainage systems to perturbations from surface meltwater inputs, with knock-on effects for glacier stability. Ultimately, our work provides an improved understanding of how surface-bed hydrological pathways may influence the future evolution of the Antarctic Ice Sheet in a warming climate.

How to cite: Hayden, A.-M., Dow, C., Hill, T., Ehrenfeucht, S., and Pelle, T.: Modelling subglacial responses to future moulin inputs in the Amundsen Sea Embayment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14926, https://doi.org/10.5194/egusphere-egu26-14926, 2026.

EGU26-14928 | ECS | Orals | CR2.3

A mixed-bed subglacial hydrology model applied to the Antarctic Ice Sheet 

Matthias Scheiter, Violaine Coulon, and Frank Pattyn

A significant part of the uncertainty of the future contribution of the Antarctic ice sheet to sea-level rise stems from unknown subglacial conditions such as geology and water content. Sliding at the base of the ice sheet depends on geological conditions, as water routing differs between soft and hard beds regions. However, ice sheet modelling studies usually do not distinguish between these different types of bed properties and instead assume it to be constant across the model domain. Also, current subglacial hydrology models have a high computational cost and their application to ice sheet models is often limited to the initialization stage.

A recent subglacial hydrology model by Kazmierczak et al. (2024) overcomes these challenges by introducing simplifications that allow to simultaneously account for hard, soft, and mixed beds, as well as efficient and inefficient drainage. The hydrology model is computationally fast, hence it can be easily fully coupled to any ice sheet model.

In this study, we apply this new subglacial hydrology model on the Ronne-Filchner basin, which includes one quarter of all ice in Antarctica and the second-largest ice shelf world-wide. The Ronne-Filchner basin exhibits sharp contrasts in subglacial topography, geology and hydrology, making it an interesting test case for the hydrology model. Furthermore, a sharp increase in sub-shelf temperatures under the Ronne-Filchner ice shelf has been suggested in coming centuries, yet this basin has been comparatively understudied thus far. We present projections under different warming scenarios and subglacial conditions, aiming to provide a sensitivity analysis of these different factors, and their interactions, on future sea level change. Our results provide insight on the importance of a detailed inclusion of subglacial geology and water evolution in large-scale ice sheet models.

 

How to cite: Scheiter, M., Coulon, V., and Pattyn, F.: A mixed-bed subglacial hydrology model applied to the Antarctic Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14928, https://doi.org/10.5194/egusphere-egu26-14928, 2026.

EGU26-14990 | ECS | Posters on site | CR2.3

Intra-annual evolution of ponded crevasses across the Greenland Ice Sheet 

Wensong Zhang, Lin Liu, Michiel van den Broeke, Bert Wouters, Xingyu Xu, Yuhan Wang, and Kang Yang

Ponded crevasses on the Greenland Ice Sheet impact the retention and drainage of surface meltwater in the low elevation zone and enhance the melt of ice sheet. However, current understanding is limited to a few glaciers, leaving their inter- and intra-annual evolution largely unknown at an ice-sheet-wide scale. This study presents an automated methodology to map ponded crevasses from 10-m resolution Sentinel-2 satellite images to produce the first pan-Greenland dataset describing their intra-annual evolution during the warm 2019 melt season. The results indicate that: 1) the central-western and southwestern basins exhibit earlier drainage onsets, due to the high surface meltwater runoff in the early melt season; 2) local topographic depressions favor higher areal expansion and shrinking rates of ponded crevasses; 3) towards the end of the melt season, a considerable amount of ponded crevasse area remains (~10% relative to the peak), suggesting the possible retention. We will further apply the proposed method to the Sentinel-2 images from 2016 to 2025 to reveal how the intra-annual evolution of ponded crevasses responds to varying climatological settings.

How to cite: Zhang, W., Liu, L., van den Broeke, M., Wouters, B., Xu, X., Wang, Y., and Yang, K.: Intra-annual evolution of ponded crevasses across the Greenland Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14990, https://doi.org/10.5194/egusphere-egu26-14990, 2026.

EGU26-14994 | ECS | Posters on site | CR2.3

Reproducing seasonal patterns of surface velocity with a coupled ice flow and subglacial hydrology model 

Annegret Pohle and Andy Aschwanden

The evolution of the subglacial drainage system plays a key role in the seasonal behavior of ice surface velocities both on mountain glaciers and ice sheets. This relationship offers an opportunity to evaluate subglacial hydrology models against observations of large spatial and temporal coverage. Although surface velocities are only an indirect measure of the subglacial water pressure, and such a comparison therefore requires the coupling to an ice flow model through a sliding law, it presents a promising but currently still under-explored opportunity for the challenging task of constraining subglacial hydrology models.

In this study, we test a coupled ice flow and subglacial hydrology model in its ability to reproduce observed patterns of seasonal surface velocity on a group of land-terminating glaciers in southwest Greenland. These glaciers exhibit a variety of seasonal behaviors, including a spring acceleration with constant winter speed, a pronounced speed minimum in autumn, as well as a sustained speed-up throughout the winter. We use the Glacier drainage system model GlaDS, coupled to a higher-order ice flow model in a way that the whole system of equations is solved simultaneously, which allows an immediate two-way coupling. While the original GlaDS is restricted to constant winter water pressures (and velocities), we explore model extensions such as a laminar/turbulent transition that yield more complex seasonal behaviors. We investigate the interplay of the physical model choices, model parameters, properties of the bed topography, meltwater input and other factors to determine which conditions are necessary to produce certain types of seasonal behavior, and we evaluate if the observed patterns can be reproduced successfully in a realistic modeling framework.

How to cite: Pohle, A. and Aschwanden, A.: Reproducing seasonal patterns of surface velocity with a coupled ice flow and subglacial hydrology model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14994, https://doi.org/10.5194/egusphere-egu26-14994, 2026.

EGU26-15205 | ECS | Posters on site | CR2.3

Observations of ice-stream velocity variability associated with subglacial lake activity in Antarctica 

Hameed Moqadam and Ingo Sasgen

Active subglacial lakes beneath the Antarctic Ice Sheet undergo repeated filling and drainage cycles that are now routinely identified using satellite altimetry. Recent studies have shown that such lakes are widespread and dynamically active, with more than few dozen active systems detected across Antarctica (Wilson et al., 2025). Even though these lakes are expected to influence basal water pressure, their impact on surface ice-stream velocity are inadequately constrained by observations.
In this study, we examine whether subglacial lake fill and drain events cause measurable, time-lagged changes in ice-stream surface velocity. The analysis focuses on a few well-documented active subglacial lakes located near major ice streams. Surface elevation time series from CryoSat-2 are used to identify lake filling and drainage phases and to quantify the timing and magnitude of individual events, also with ICESat-2 data used for validation where available. Ice velocity time series derived from Sentinel-1 are extracted at multiple locations upstream and downstream of each lake and are detrended to isolate velocity anomalies.
We analyse the relationship between lake elevation changes and velocity anomalies using correlation and lead lag methods, and assess how any velocity response varies with distance from the lake. Statistical significance is evaluated relative to background velocity variability and sensitivity to spatial averaging. The results provide observational constraints on the coupling between subglacial hydrology and ice dynamics, and help to assess whether subglacial lake activity can produce detectable surface velocity responses at satellite resolution.

 

Wilson, S.F., Hogg, A.E., Rigby, R. et al. Detection of 85 new active subglacial lakes in Antarctica from a decade of CryoSat-2 data. Nat Commun 16, 8311 (2025). https://doi.org/10.1038/s41467-025-63773-9

How to cite: Moqadam, H. and Sasgen, I.: Observations of ice-stream velocity variability associated with subglacial lake activity in Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15205, https://doi.org/10.5194/egusphere-egu26-15205, 2026.

EGU26-16195 | ECS | Orals | CR2.3

Ice surface steepening drives multi-decadal acceleration of the Greenland Ice Sheet interior 

Hannah Picton, Andrew Tedstone, Peter Nienow, Horst Machguth, Dan Goldberg, Nicolas Jullien, Nicole Clerx, Christoph Posch, Marcus Gastaldello, and Dirk van As

Annual ice flow along the land-terminating margins of the Greenland Ice Sheet has been negatively correlated with surface melt over recent decades, a trend commonly attributed to the seasonal evolution of efficient subglacial drainage in response to larger melt volumes. However, there remains scant observational evidence of ice flow behavior at higher elevations in the accumulation zone, despite increasing surface melt and runoff. Here, we employ in-situ GPS measurements to analyse multi-decadal (1996-2023) variations in ice motion and surface slope along the land-terminating K-Transect, West Greenland, between ~ 1400 and ~ 1900 m.a.s.l.

We show that below the equilibrium line altitude (ELA), annual ice motion is negatively correlated with surface melt, consistent with the self-regulation of ice flow previously reported across the ablation zone. In contrast, above the ELA, we observe a small but persistent ice flow acceleration, punctuated by slowdowns in the large melt years of 2012 and 2023. We find that this ice flow acceleration has largely been driven by surface steepening, with the resultant increase in driving stress calculated to account for 70.0 ± 26.7% of the acceleration observed at ~ 1700 m.a.s.l. between 2009 and 2021. However, together with continued muted seasonality in ice flow at ~ 1900 m.a.s.l. already identified during 2009-2012, we also find clear evidence of direct surface meltwater access to the ice sheet bed at ~ 1700 m.a.s.l for the first time in our observation record. It is therefore possible that the drainage of surface meltwater has driven some of the observed acceleration, through increasing the basal sliding component of ice flow.

With the rate of ice surface lowering at the ice sheet margin predicted to continue to exceed that in the ice sheet interior, we expect that ice surface steepening will likely persist, thereby driving sustained ice flow acceleration across the higher elevations in the coming years. The direct impact of this ice flow acceleration on mass loss by drawdown will likely be modest; whilst increased ice will be advected to lower elevations where air temperatures are higher, downstream self-regulation of ice flow is expected to constrain the resultant increase in ice flux. However, our findings show that surface-to-bed connections can form above the ELA, which has implications for the volume and timing of runoff from the high elevation regions which undergo summer melt increasingly often.

How to cite: Picton, H., Tedstone, A., Nienow, P., Machguth, H., Goldberg, D., Jullien, N., Clerx, N., Posch, C., Gastaldello, M., and van As, D.: Ice surface steepening drives multi-decadal acceleration of the Greenland Ice Sheet interior, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16195, https://doi.org/10.5194/egusphere-egu26-16195, 2026.

EGU26-17759 | ECS | Orals | CR2.3

Meltwater Drainage in Troughs Controls end-of-summer Regional Ice Flow Deceleration in Western Greenland 

Jonas Kvist Andersen, Florent Gimbert, and Benjamin Joseph Davison

The subglacial drainage system of the Greenland Ice Sheet plays a central role in modulating basal sliding and ice flow dynamics. While the seasonal evolution of this system has been widely studied during the melt season onset, its late and post-melt season behavior remains poorly constrained due to limited spatial and temporal observational coverage. Here, we use Sentinel-1 double-difference interferometric SAR data to document spatially continuous patterns of vertical and horizontal ice sheet motion across the late melt season in a predominantly land-terminating region of western Greenland. Our observations reveal recurrent, localized vertical subsidence features, generally coinciding with subglacial troughs, that persist several weeks into the post-melt season (late August to October) after surface melt inputs have largely ceased. The localized subsidence signals are accompanied by ice flow deceleration at a regional scale, extending more than 100 km inland, to ice thicknesses above 1300 m. We interpret this pattern as a dynamic response to the gradual drainage of water stored in weakly-connected cavities or, alternatively, englacial or sedimentary components, which drives a large-scale water pressure decrease and hence widespread flow deceleration. Although prior studies have suggested that weakly-connected cavities are drained following de-pressurization of efficient channels, the multi-week time scale and far-inland extent of the observed dynamic response suggest that channels may not be the sole driving mechanism. The magnitude of both subsidence and slow-down scales with melt season intensity, suggesting a mechanistic link between meltwater drainage efficiency and late-season ice dynamics, in line with previous observations of ice flow self-regulation. Our findings offer new insights into the seasonal evolution of Greenland's basal hydrology with continuous spatial coverage, highlighting how localized corridors of meltwater evacuation affect ice motion over much larger scales. 

How to cite: Andersen, J. K., Gimbert, F., and Davison, B. J.: Meltwater Drainage in Troughs Controls end-of-summer Regional Ice Flow Deceleration in Western Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17759, https://doi.org/10.5194/egusphere-egu26-17759, 2026.

EGU26-19022 | ECS | Posters on site | CR2.3

Reactivation of lateral meltwater export from Bach Ice Shelf following a 9-year hiatus 

Rebecca Dell, Michelle Maclennan, Luke Trusel, and Mahsa Bahrami

Since the 1950’s ice-shelf surface meltwater has been implicated as a driver of partial and complete collapse events across several ice shelves on the Antarctic Peninsula. Many of these events occurred alongside marked increases in 2m air temperatures in the later half of the 20th century, which drove increased rates of surface melting. Whilst this warming was briefly punctuated by a partial cooling across the Antarctic Peninsula from 1999 to 2014, it has since resumed. Given projections of non-linear increases in surface melting under future climate scenarios, surface meltwater-driven instabilities become increasingly important. Whilst most studies to date have focussed on the potential for hydrofracture, it is important that we begin to consider the potential for ice-shelf run-off and lateral meltwater export as Antarctica progresses towards Greenlandification. 

Here we present remotely sensed evidence for the re-initiation of surface meltwater export from Bach Ice Shelf, following a 9-year hiatus.  We combine optical remote sensing (Landsat 7, 8, and 9) with 43 years of regional climate model outputs (RACMO2.3p2 and ERA5) to evidence this change and consider the climate conditions that may have driven it. Variables considered include modelled surface mass balance, melt, and 2 m air temperatures. Melt-to-SMB ratios were calculated from modelled surface mass balance and melt. 

In the austral summer of 2022/23, lateral meltwater export resumed on Bach Ice Shelf, ending the observed 9-year hiatus. This hiatus may have been driven by high surface mass balance and low snowmelt values, which resulted in low melt-to-SMB ratios. Such low melt-to-SMB ratios likely increased ice-shelf firn air content, which then took several years to overcome. The return of lateral meltwater export from Bach Ice Shelf in 2022/23 coincided with the highest modelled mean annual 2 m air temperatures. With continued atmospheric warming, we anticipate that Bach’s meltwater regime will continue to exhibit lateral meltwater export in the future, demonstrating the renewed importance of surface run-off for ice shelves on the Antarctic Peninsula. 

How to cite: Dell, R., Maclennan, M., Trusel, L., and Bahrami, M.: Reactivation of lateral meltwater export from Bach Ice Shelf following a 9-year hiatus, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19022, https://doi.org/10.5194/egusphere-egu26-19022, 2026.

EGU26-20314 | Posters on site | CR2.3

Canals: distributed versus channelised 

Mauro Werder and Ivan Utkin

Subglacial drainage through ice and sediment incised channels, so-called canals, likely impacts the dynamics of soft bedded glaciers and ice streams as well as dictating sediment evacuation from ice sheet and glaciers. The original work of Walder and Fowler (1993) found that canals would form a distributed drainage system, i.e. that many small canals would be favoured over one large canal for a given discharge. We present a simple 1D numerical canal model which simulates both ice and sediment incision, water flow and sediment transport whilst assuming a fixed shape of the channel. With this model we investigate the distributed vs channelised behaviour of canals and extract which processes impact this dichotomy.

How to cite: Werder, M. and Utkin, I.: Canals: distributed versus channelised, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20314, https://doi.org/10.5194/egusphere-egu26-20314, 2026.

EGU26-20359 | ECS | Posters on site | CR2.3

Widespread lake-terminating glacier slowdown despite ice-marginal lake expansion in Greenland 

Yefan Wang, Peter Nienow, Jaime Otero, and Daniel Goldberg

Accelerated global warming is driving significant mass loss from the Greenland Ice Sheet (GrIS), leading to widespread ice-margin retreat and increased meltwater runoff. Both processes have resulted in a widespread increase in the number, area, and volume of ice-marginal lakes. These proglacial water bodies are known to possess significant potential to influence ice motion and, thus, ice sheet stability by altering thermal and mechanical boundary conditions at the terminus. Consequently, there is an imperative to understand how recent expansions in lake extent have impacted ice dynamics around the margins of the GrIS.

In this study, we investigate changes in near-terminus ice dynamics for the 76 glaciers draining into the 70 largest ice-marginal lakes around the GrIS over a 25-year period (1999–2024). We analyze velocity variation within the near-terminus region to isolate the direct influence of the ice-marginal lake. The results show that the studied glaciers have experienced an overall slowdown in ice motion of 19% between 1999 and 2024. While we observe regional variability across the ice sheet, no individual sector exhibits aggregate acceleration. Overall, only 32% of the studied glaciers accelerated in their near-terminus region. In these specific instances, speed-up is driven primarily by ice-marginal thinning and/or proglacial lake deepening, both of which increase flotation and consequently reduce basal drag.

These findings challenge the prevailing view that ice-marginal lake growth inevitably promotes dynamic instability. While ice-marginal lakes are increasing around the GrIS, we find no evidence over the last 25 years that these systems are making an increasing contribution to ice mass loss via ice dynamics. This suggests that many ice-marginal lakes lack the depth or overdeepened bed topography necessary to induce significant flotation-driven instability.

How to cite: Wang, Y., Nienow, P., Otero, J., and Goldberg, D.: Widespread lake-terminating glacier slowdown despite ice-marginal lake expansion in Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20359, https://doi.org/10.5194/egusphere-egu26-20359, 2026.

EGU26-21093 | ECS | Orals | CR2.3

Elliptical Röthlisberger Channels: Modelling Flow, Heat and Evolution 

Isaac Brown, Katarzyna Warburton, and Jerome Neufeld

Subglacial water flow plays a critical role in basal sliding and, consequently, in glacier and ice-sheet dynamics. However, modelling the coupled evolution of subglacial drainage and ice flow remains challenging. This study investigates the evolution of the basal ice–water interface by analysing heat and fluid flow in idealised englacial channels. We extend the classical Röthlisberger model for circular channels to elliptical channel geometries. A hybrid turbulent–laminar melt scheme captures heat generation from both viscous and turbulent dissipation, while a viscous flow law models the creep closure of the surrounding ice. The flow and temperature profiles in elliptical channels are solved for with differential melting between the roof and walls of the channel. We find that elliptical channels tend towards a circular shape when laminar melting dominates, whilst the flow of ice tends to increase the eccentricity of the channel. Our hybrid laminar-turbulent melt model permits variations in the distribution of melting along the ice-water boundary and the existence of stable, non-circular cross-sections. These stable channels obey pressure-flux relationships that we use to explore the evolution and dynamics of hydrologically interacting channels in a wider subglacial drainage network, working towards a simplified and scalable subglacial hydrology model.

How to cite: Brown, I., Warburton, K., and Neufeld, J.: Elliptical Röthlisberger Channels: Modelling Flow, Heat and Evolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21093, https://doi.org/10.5194/egusphere-egu26-21093, 2026.

EGU26-878 | ECS | Posters on site | CR2.4

Modelling the influence of thermal state and sliding on the dynamics of Grenzgletscher, Swiss Alps 

Cristina Gerli, Elisa Mantelli, and Thomas Zwinger

Alpine glaciers provide an accessible window into the dynamics of Antarctic ice streams, providing key insights into the processes controlling ice flow. Grenzgletscher, a polythermal glacier in the Swiss Alps, has cold-bedded ice in the accumulation zone and temperate-bedded ice downstream. The location of the transition between these basal regimes remains poorly constrained. We build a full-Stokes ice flow model with Elmer/Ice to reproduce observed surface velocities under varying basal conditions. Three scenarios are tested: (1) a frozen bed (no slip); (2) sliding with spatially variable basal friction; and (3) inclusion of borehole-derived temperature profiles to evaluate the influence of thermal structure on flow. The study provides constraints for geophysical investigations where surface velocities are not matched and informs a borehole campaign planned for next summer targeting the cold-temperate transition. These simulations aim to clarify how basal thermal state and sliding jointly shape glacier dynamics.

How to cite: Gerli, C., Mantelli, E., and Zwinger, T.: Modelling the influence of thermal state and sliding on the dynamics of Grenzgletscher, Swiss Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-878, https://doi.org/10.5194/egusphere-egu26-878, 2026.

EGU26-1137 | ECS | Orals | CR2.4

Temporal ice-stream dynamics resulting from subtemperate sliding instabilities 

Tilly Woods, Elisa Mantelli, Thomas Zwinger, and Christian Schoof

Ice streams are fast-flowing “rivers” of ice within an ice sheet, and are responsible for the majority of mass loss from continental ice sheets. The onset region of these ice streams is especially interesting, as that is where ice transitions from slow interior flow to fast, sliding-dominated ice-stream flow. Subtemperate sliding, i.e., sliding below the melting point, is thought to be important in enabling this transition. Previous theoretical work has shown that the subtemperate region is subject to a host of temporal instabilities. Yet, the role of these instabilities in driving the temporal dynamics of ice streams remains unclear. In this work, we use a thermomechanically-coupled Stokes flow model of an idealised, 2D ice-sheet flowline in Elmer/Ice to investigate how these temporal linear instabilities play out in the full nonlinear evolution of the ice sheet. Using a combination of numerical simulations and theory allows us to investigate the physical mechanisms behind sliding onset, and to gain insight into what controls the observed switching “on and off” of ice streams over time. We also explore details of a thermodynamically consistent numerical implementation in Elmer/Ice of frozen-temperate boundaries at the bed.

How to cite: Woods, T., Mantelli, E., Zwinger, T., and Schoof, C.: Temporal ice-stream dynamics resulting from subtemperate sliding instabilities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1137, https://doi.org/10.5194/egusphere-egu26-1137, 2026.

EGU26-1602 * | ECS | Orals | CR2.4 | Highlight

What does marine ice sheet (in)stability mean in the context of climate overshoot? 

Alexander Bradley and Felicity McCormack

In the classical marine ice sheet instability, a grounding line of an unbuttressed ice sheet on a retrograde bedslope (that is, upwards sloping in the direction of ice flow) is theoretically unstable. However, these theories assume that the forcing on the ice sheet changes slowly, compared to the timescale on which the ice sheet responds to climate perturbations. In a world where climate forcing is ramping up very quickly, this assumption probably doesn’t hold. This is particularly pertinent in the context of climate overshoots — temporary detours above the 1.5C Paris Agreement target — which look increasingly likely if we are to ultimately limit warming to 1.5C. For how long, and how far, can we overshoot 1.5C, while avoiding passing a tipping point, even if that tipping point is around 1.5C of warming? We probe these questions using a simple model of grounding line dynamics, in conjunction with few, more detailed simulations of the retreat of the Pine Island Glacier over the 20th century following its passing a tipping point. We demonstrate that temporary overshoots above tipping points are possible, provided that climate forcing is ramped down sufficiently quickly. However, the likelihood of extreme ice loss is very sensitive to how high the overshoot goes, demonstrating the need to limit overshoots to prevent significant, long timescale ice loss from the Antarctic Ice Sheet. 

How to cite: Bradley, A. and McCormack, F.: What does marine ice sheet (in)stability mean in the context of climate overshoot?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1602, https://doi.org/10.5194/egusphere-egu26-1602, 2026.

EGU26-1647 | ECS | Posters on site | CR2.4

 Modelling glacial and periglacial processes in the Karkonosze Mountains 

Marta Sadkiewicz and Marek Kasprzak

The Karkonosze Mountains are one of the few ranges within the Bohemian Massif that preserve evidence of Pleistocene glaciations. They also constitute an area where some of the earliest investigations into mountain glaciation and the processes now referred to as periglacial were undertaken. Despite the relatively good geomorphological understanding of the Karkonosze, the abundance of environmental studies, and the broad availability of digital datasets, a clear synthesis remains lacking, not only regarding the age of the former glaciers, but also their extent and thickness. Changes in the altitudinal zones in which periglacial processes operated during the Pleistocene and Holocene have likewise not been examined. In this study, we re-evaluate the existing literature and available rock- and sediment-dating data. We conduct a detailed analysis of a high-resolution Digital Terrain Model (DTM) using GIS-based methods. The results enable a partial reconstruction of the extent of the Karkonosze glaciers and allow us to determine the spatial range and duration of the periglacial zone. The landforms shaped by these processes are fundamental to the distinctive character of the Polish and Czech national parks in the region, and knowledge of their origin should be communicated effectively to a broader audience.

 

How to cite: Sadkiewicz, M. and Kasprzak, M.:  Modelling glacial and periglacial processes in the Karkonosze Mountains, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1647, https://doi.org/10.5194/egusphere-egu26-1647, 2026.

EGU26-1854 | ECS | Posters on site | CR2.4

Evaluating calving functions: emergent dynamics from a position-based calving function and the limits of rate-based calving functions.  

Iain Wheel, Doug Benn, Anna Crawford, and Samuel Cook

A wide range of calving functions is currently available but there is no consensus on the best approach. Current assessments of calving functions are often crudely done by fitting functions to observed terminus positions, neglecting the physical processes that drive changes in calving dynamics. Here, we use 3D simulations of synthetic tidewater glacier domains in Elmer/Ice, to determine whether natural behaviours emerge from the crevasse-depth and von Mises calving functions, and to provide a basis for more robust assessments of the potential capabilities of calving functions. Both functions are derived from the full 3D Cauchy stress tensor and are simple functions that can be exported to ice sheet models. The crevasse-depth calving function is shown to be able to simulate both serac and full thickness calving events and simulates how their relative proportion is altered by changing the ice freeboard or submarine melting. A clear distinction between rate- and position-based calving is shown with the von Mises calving function unable to respond to imposed changes in topography or glacier geometry. Importantly, any feedback between glacier dynamics and the von Mises calving function is through an unphysical velocity feedback loop.  

Through these simple experiments we show both steady state and transient behaviour can modelled using a position-based calving function while rate-based functions can only capture an imposed state. It is clear we must look beyond just terminus positions when assessing the suitability of a calving function. Manual tuning can mask unphysical calving behaviour and restrict behaviour to that of the tuned period. Furthermore, we show that a robust calving function does not require site or timeframe specific tuning using the crevasse-depth calving function at Store Glacier (Sermeq Kujalleq) and Jakobshavn Isbrae (Sermeq Kujalleq). 

By comparing the two calving functions, it is apparent that full-depth calving is irrefutably position-based. Consequently, future projections must not be made using rate-based calving functions. Using a position function, calving rates vary with time and glacier state, so cannot be assumed to be a constant function of stress. 

How to cite: Wheel, I., Benn, D., Crawford, A., and Cook, S.: Evaluating calving functions: emergent dynamics from a position-based calving function and the limits of rate-based calving functions. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1854, https://doi.org/10.5194/egusphere-egu26-1854, 2026.

EGU26-1931 | ECS | Orals | CR2.4

A viscoelastic phase-field model for calving and fracture in ice  

Daniel Richards, Robert Arthern, and Oliver Marsh

Iceberg calving due to fracture accounts for around half of the ice lost annually from Antarctica, but physically based models representing this process are not currently included in ice sheet models. By using a phase-field viscoelastic model for fracture we can model both slow deformation of ice and the distribution and evolution of cracks leading to calving. The model solves equations for non-linear viscous flow, elastic displacement and a phase-field variable which allows cracks to nucleate and propagate in response to the evolving stress field. Without making any assumptions about the type of calving, we apply this model to a simulate fracture of an iceberg. We explore how the calving rate is influenced by changing a range of parameters, and find it is particularly sensitive to the water level inside the cracks.  

How to cite: Richards, D., Arthern, R., and Marsh, O.: A viscoelastic phase-field model for calving and fracture in ice , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1931, https://doi.org/10.5194/egusphere-egu26-1931, 2026.

EGU26-2036 | Orals | CR2.4

Machine-learned global glacier ice volumes 

Niccolò Maffezzoli, Eric Rignot, Carlo Barbante, Mathieu Morlighem, Troels Petersen, and Sebastiano Vascon

Knowledge of glacier ice volumes is crucial for constraining future sea level rise, evaluating freshwater resources, and assessing impacts on societies, from regional to global. Yet, significant uncertainties persist in both regional estimates of total glacier ice volume and in distributed ice thickness for individual glaciers. Here, we present the results from IceBoost v2.0, a machine learning system able to model the ice thickness of individual glaciers, trained on 7 million ice thickness measurements and informed by physical and geometrical predictors. Globally, we find a total glacier volume of (149 ± 38) × 103 km3 and sea level equivalent of 323 ± 91 mm, both well within existing estimates. We examine major glaciated regions and compare the results with other models. Confidence in our solution is highest at higher latitudes, where abundant training data adequately sample the feature space. Over steep and mountainous terrain, small glaciers, and under-represented lower-latitude regions, confidence is lower. IceBoost v2.0 demonstrates strong generalization at ice sheet margins. On the Geikie Plateau, East Greenland, we find nearly twice as much ice compared to BedMachine v3, highlighting the method's potential to refine the bed topography in parts of the ice sheets. The quality of the modeled ice thickness depends on the accuracy of the training data, the digital elevation model, ice velocity fields, and glacier geometries, including nunataks. We present the released dataset of ice thickness and associated uncertainty for all glaciers within the Randolph Glacier Inventory version 6 and 7, totaling half a million maps. This may be useful for modeling glacier dynamics, future evolution and sea-level rise, informing the design of glaciological surveys, field campaigns, as well as guiding policies on freshwater management.

How to cite: Maffezzoli, N., Rignot, E., Barbante, C., Morlighem, M., Petersen, T., and Vascon, S.: Machine-learned global glacier ice volumes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2036, https://doi.org/10.5194/egusphere-egu26-2036, 2026.

EGU26-3127 | ECS | Posters on site | CR2.4

Modelling Subglacial Blisters and Transient Ice-Flow Anomalies Following Supraglacial Lake Drainage 

Hanwen Zhang, Laura Stevens, Ian Hewitt, and Harry Stuart

On the Greenland Ice Sheet, drainage of supraglacial lakes via hydrofracture can transport substantial volumes of meltwater into the subglacial drainage system within hours, generating subglacial “blisters” that transiently accelerate adjacent ice flow. The blisters subsequently dissipate, with their thickness diminishing as water spreads laterally, propagates, and leaks into adjacent components of the subglacial drainage system. Although field observations reveal surface-elevation and velocity anomalies associated with blisters, existing subglacial hydrology models—typically comprised of linked cavities and channels—do not include the physics of elastic ice uplift, and therefore cannot reproduce the observed flood propagation or ice-flow anomalies.

We present a modelling framework that integrates elastic ice uplift with an established subglacial hydrology model of linked cavities and channels to model subglacial blisters and their interactions with the surrounding hydrological network. We further couple this framework to a depth-integrated ice-flow model, and simulate the resulting, transient surface-uplift and velocity anomalies following lake drainages. This unified model provides a new tool for interpreting remote-sensing and in situ observations of drainage events on short timescales, and for assessing how lake-drainage processes influence ice dynamics and the long-term mass balance of the Greenland Ice Sheet.

How to cite: Zhang, H., Stevens, L., Hewitt, I., and Stuart, H.: Modelling Subglacial Blisters and Transient Ice-Flow Anomalies Following Supraglacial Lake Drainage, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3127, https://doi.org/10.5194/egusphere-egu26-3127, 2026.

EGU26-3526 * | ECS | Orals | CR2.4 | Highlight

The perimeter feedback: a cornerstone of ice-sheet stability 

Jan Swierczek-Jereczek, Jorge Alvarez-Solas, Alexander Robinson, Lucía Gutiérrez-González, and Marisa Montoya

Ice sheets can undergo self-sustained retreat (or regrowth), with important impacts on sea-level, climate and consequently life on Earth. For instance, the collapse of the ice saddle between the Cordilleran and the Laurentide Ice Sheet during the last deglaciation has been suggested to contribute to the rapid sea-level rise that characterized Meltwater Pulse 1A, which led to significant changes in atmospheric circulation thereafter. Conversely, saddle mergers have been shown to drive self-sustained ice growth, potentially playing a key role in the large-scale inception of the Laurentide and British Isles Ice Sheet. In the present work, we simulate a similar behaviour for the Antarctic Ice Sheet, which additionally presents a larger hysteresis and more bifurcation points than previously simulated. We generalise the idea of saddle merger/collapse under the concept of perimeter feedback, which applies well beyond this specific case and refers to the fact that an ice sheet typically increases its mass balance when decreasing the ratio of perimeter to surface area. This is largely conditioned by the bedrock roughness and the coastline irregularity, and results from the interplay between thermo-mechanics, ice-ocean-atmosphere interactions and geometry. In particular, we show that the perimeter feedback plays a key role in the collapse of the West-Antarctic Ice Sheet simulated under global warming, as well as in abrupt regrowth of the East-Antarctic Subglacial Basins under global cooling. The analysis performed here does not introduce new physics but provides a key tool to better understand a ubiquitous mechanism underlying the instabilities simulated by ice-sheet models.

How to cite: Swierczek-Jereczek, J., Alvarez-Solas, J., Robinson, A., Gutiérrez-González, L., and Montoya, M.: The perimeter feedback: a cornerstone of ice-sheet stability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3526, https://doi.org/10.5194/egusphere-egu26-3526, 2026.

Iceberg calving from tidewater glaciers has contributed more than half of the total mass loss of the Greenland Ice Sheet over the past four decades, and observations have shown that episodes of increased iceberg discharge have coincided with rising air temperatures and/or the occurrence of warmer coastal waters into fjords within which they discharge. Despite significant advances in understanding over the last two decades, major uncertainties still remain in understanding how sensitive iceberg calving rates are to climate-induced exchanges of heat and freshwater around marine terminating ice sheet margins. This is partly because we do not know the long-term, multi-decadal to centuries historical context of the ice-ocean system that links our understanding of contemporary process with longer term glacier response to climate. 

In this study, we use the Ice-sheet and Sea-level System Model (ISSM) to simulate the advance and retreat of a fast-flowing tidewater glacier in southwest Greenland, Kangiata Nunata Sermia, over the last 1000 years to indentify the drivers of advance and retreat and evaluate calving-parameter choices against observed long-term ice-margin variability. While models have successfully reproduced observed recent retreat, their parameters are rarely tested against centennial- to millennial-scale records of advance. We explore the parameter space governing calving-front advance, focusing on submarine melt rates and von Mises calving-law stress thresholds for grounded and floating ice and validate model ensembles against a well-constrained millennial-scale record of advance and retreat. Using Latin Hypercube Sampling, we assess two criteria: whether the calving front advances at all, and whether it can reach the reconstructed Little Ice Age (LIA) position. 

We find that advance can occur across the full tested range of submarine melt rates, up to 1.5 m d⁻¹. However, successful advance to the LIA position is more tightly constrained by the von Mises stress thresholds. In several simulations, the calving front advances only as far as a widening in the fjord, unless the calving rate is reduced by setting a sufficiently high stress thresholds. Our results highlight a strong interaction between calving physics and fjord geometry in controlling long-term advance. This project contributes to improving confidence in multi-decadal to centennial projections of ice sheet behaviour through validating model performance over similar timescales including prolonged episodes of both glacier advance and retreat. 

How to cite: Jones, D., Mair, D., Nias, I., Lea, J., and Morlighem, M.: Modelling the advance and retreat of major Greenlandic tidewater glacier over the last 1000 years reveals high sensitivity to calving front forcing criteria, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3545, https://doi.org/10.5194/egusphere-egu26-3545, 2026.

EGU26-3787 | Orals | CR2.4

A novel approximation for the flow of ice in narrow valleys 

Stefan Hergarten

Recently, a very efficient numerical scheme for the shallow ice approximation (SIA) was proposed. It technically even allows for 0.25 year time increments at spatial resolutions of 25 m, which would make it a very interesting tool for simulating alpine glaciers. However, the SIA in its simplest form neglects all horizontal stress components, which leads to severe limitations in alpine valleys, where the ice thickness is typically not sufficiently small compared to the valley width. The question of whether there is a chance to extend the new numerical scheme to more complex flow models remained open.

Here, preliminary tests of an approach that somehow builds a new house from the roof are presented. The idea is not to include the additional terms of existing extensions of the SIA (e.g., second-order terms or a combination with the shallow shelf approximation) in the numerical scheme, but to develop a new approximation to the Stokes equations that already harmonizes well with the new numerical scheme. As a key point, the basic structure of the SIA is kept in the sense that ice flow still follows the steepest decline of the ice surface (hydrostatic approximation). In turn, the diffusivity term of the SIA is no longer parameterized directly by the ice thickness and the slope, but described by an additional differential equation. This differential equation is developed explicitly for taking into account the transverse shear stresses, which contribute much to the deficiencies of the SIA in narrow alpine valleys.

The first results, obtained from 2-D simulations of valley cross sections, are very promising. The additional differential equation can be parameterized in such a way that the error in total ice flux is only a few percent for various valley shapes even down to aspect ratios of 2:1. The across-valley profile of the surface velocity is also reproduced quite well as long as sliding is not too strong. As a main limitation, however, longitudinal stress components cannot be included easily.

How to cite: Hergarten, S.: A novel approximation for the flow of ice in narrow valleys, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3787, https://doi.org/10.5194/egusphere-egu26-3787, 2026.

EGU26-4251 | Orals | CR2.4

Progress in understanding and modelling calving 

Douglas Benn, Iain Wheel, Jan Åström, Adrian Luckman, Samuel Cook, Poul Christoffersen, Will Spicer, and Faezeh Nick

The importance of calving losses from marine-terminating ice margins in a warming world has highlighted the need for reliable representation of calving in predictive ice-sheet models. However, there is currently no consensus regarding the most appropriate form for calving functions (so-called 'calving laws'), and the calving problem remains open. We advocate an integrated approach, in which observations, theory and high-fidelity modelling are used to develop and calibrate optimal, general calving functions for continuum ice-sheet models. Our work has demonstrated that calving is a stochastic process that gives rise to self-organising behaviour at a range of scales, including calving-size distributions, waiting times, and ice-front fluctuations. Individual calving events occur in response to critical and/or sub-critical crack propagation under tensile, shear or mixed stress regimes. We have used these insights to develop a position-based stochastic calving function, in which calving probabilities are scaled to the state of stress in the ice. When implemented in the full-stress continuum model Elmer/Ice, the calving function exhibits a wide range of realistic self-organising behaviour, and successfully reproduces observed ice-front fluctuations of Jakobshavn Isbrae and Store Glacier without the need for site-specific tuning. A calving algorithm suitable for vertically integrated ice-sheet models is in development.  

How to cite: Benn, D., Wheel, I., Åström, J., Luckman, A., Cook, S., Christoffersen, P., Spicer, W., and Nick, F.: Progress in understanding and modelling calving, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4251, https://doi.org/10.5194/egusphere-egu26-4251, 2026.

EGU26-4612 | Posters on site | CR2.4

When the Ground and the Glacier Disagree: The Timing Mystery of Bedrock Uplift and Ice Discharge Peaks 

Gong Cheng, Valentina R. Barletta, Danjal Berg, Mathieu Morlighem, Shfaqat Abbas Khan, and Helene Seroussi

Accurate partitioning of present-day Greenland Ice Sheet (GrIS) mass change is essential for closing the sea-level budget and constraining future projections. Vertical bedrock motion from the Greenland GNSS Network (GNET) has recently been used as a virtual instrument for GrIS mass change, but interpretations diverge. At Jakobshavn Isbræ, GNSS uplift has been linked both to dynamic thinning that leads changes in ice discharge by about 0.87 years, implying predictive power for future ice flux, and to seasonal uplift peaks that precede ice-mass loss by 4.5–9 weeks, interpreted as evidence for substantial transient meltwater storage within the ice sheet. Here we reconcile these seemingly contradictory results by jointly analysing GNET observations, mass-balance products, and a numerical ice-sheet model of Greenland’s major outlet glaciers. We show that there is neither a phase shift between bedrock uplift and ice mass-change signals nor any substantial seasonal missing mass. Instead, we find that the two earlier results stem from an incorrect physical interpretation of the GNSS signal. From our analysis, the variability in bedrock uplift is primarily driven by the advance and retreat of the ice front within roughly 10 kilometres of the glacier termini, a zone that is often poorly captured by input–output methods and coarse-resolution mass-balance products. Our results clarify the physical origin and timing of vertical bedrock shifts in Greenland and provide tighter constraints on the contemporary GrIS mass budget.

How to cite: Cheng, G., Barletta, V. R., Berg, D., Morlighem, M., Khan, S. A., and Seroussi, H.: When the Ground and the Glacier Disagree: The Timing Mystery of Bedrock Uplift and Ice Discharge Peaks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4612, https://doi.org/10.5194/egusphere-egu26-4612, 2026.

EGU26-4960 | ECS | Orals | CR2.4

Mechanical anisotropy as a driver of shear margin and ice stream formation 

Yu Zhang, Paul D. Bons, Steven Franke, Till Sachau, Haibin Yang, Ágnes Király, and Ilka Weikusat

Fast-flowing ice streams drain most of the inland ice from the Antarctic and Greenland ice sheets (GrIS). The Northeast Greenland Ice Stream (NEGIS), for example, extends for more than 500 km from the central GrIS ice divide to its outlets, with flow velocities up to ten times higher than in the surrounding ice. Despite extensive research, the mechanisms responsible for ice stream formation remain poorly understood. NEGIS, as a representative case of ice streams that are not topographically confined, has recently also been found to lack an area of elevated geothermal heat flux below. However, no model has so far been able to test whether ice stream initiation can solely result from the evolving internal properties of the ice itself, without relying on external forcing, given that slow-moving ice may be frozen to the bed before ice-stream formation.

Ice is strongly anisotropic because it deforms more easily parallel to its crystallographic basal plane than perpendicular to it along the crystal's c-axis. During deformation, this difference leads to a preferred alignment of the crystal lattice orientations. This anisotropy has significant implications for ice flow. We present a three-dimensional full-Stokes model of an analogue to NEGIS. In our modelling, ice first shows convergent flow towards the outlet gate. During flow, c-axis rotations calculated by our model cause the directional alignment of the easy-glide crystallographic basal planes parallel to the vertical shear plane, which make the ice effectively softer. Shear zones usually form in pairs due to the localized shearing, known as shear margins that bound the ice stream that can now flow much faster and extend further inland. Our results show that a fully developed, fast-flowing ice stream can form in only 1000–2000 years solely due to the evolving ice anisotropy. We perform several model runs up to 4000 years to explore the effect of varying boundary conditions, which result in different geometries of an ice-stream system. Ice streams in the system can potentially initiate and evolve by the formation and movement of shear margins in relation to the location of outlet gates within the drainage basin. This work stresses the importance of evolving ice anisotropy on ice-sheet mass balance and sea-level rise during global climate change.

How to cite: Zhang, Y., Bons, P. D., Franke, S., Sachau, T., Yang, H., Király, Á., and Weikusat, I.: Mechanical anisotropy as a driver of shear margin and ice stream formation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4960, https://doi.org/10.5194/egusphere-egu26-4960, 2026.

The future evolution of Greenland’s remaining ice shelves is generally not considered a major contributor to the ice sheet’s overall mass loss. However, their role in buttressing the present-day ice sheet has not yet been quantified through a systematic analysis. Here we perform a series of experiments with the ice-sheet model Úa. Results from a control simulation with present-day ice shelf extents and atmospheric conditions are contrasted to RCP8.5 climate change scenario with 1) intact ice-shelves, and 2) the catastrophic and irreversible loss of all floating ice. Immediately following ice shelf collapse, ice flux across the grounding line doubles, leading to a sustained more than 4-fold increase in solid ice discharge, with implications for how freshwater flux influences local ocean circulation. By the end of the century, these end-member scenarios demonstrate a response of ~2.5 mm additional sea level rise due to ice shelf loss.

How to cite: Zanker, J. and De Rydt, J.: Assessing the Importance of Greenland's Ice Shelves for Future Sea Level Rise Predictions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5790, https://doi.org/10.5194/egusphere-egu26-5790, 2026.

EGU26-5996 | ECS | Orals | CR2.4

Quantifying the uncertainty in Greenland’s contribution to sea level rise due to the bed topography 

Mansa Krishna, Mathieu Morlighem, Danielle Mangini, and Youngmin Choi

Uncertainty in the future contribution of the ice sheets to sea level rise associated with different climate forcings has been well studied in the most recent Ice Sheet Model Intercomparison Project for CMIP6 (ISMIP6). Similarly, the uncertainty due to differences in basal sliding laws or calving laws has also been thoroughly investigated. However, the uncertainty due to the bed topography has not yet been rigorously quantified. The majority of the models within the ISMIP6 ensemble use a single bed topography map, BedMachine Greenland, thereby hindering our ability to better understand how uncertainties in the bed topography affect the overall uncertainty in future projections of sea level rise. To address this, we follow the methodology from Castleman et al. (2022) and create an ensemble of 32 bed topography maps with realistic bed roughness by perturbing the BedMachine bed topography using discrete wavelet decomposition techniques. We update the initial bed topography in ice sheet models from Choi et al., (2021), which provide Greenland-wide, high-resolution, data constrained projections that include calving dynamics, and run projections out to 2300. Though we expect northwest and central west Greenland glaciers to contribute more to sea level rise than other glaciers, we find that models initialized with BedMachine bed topographies tend to overestimate mass loss in these regions. We also find that the addition of bed roughness reduces the future contribution of the ice sheet to sea level rise over the 21st century, but to a lesser extent than the deep, wide subglacial basins of Antarctica. Lastly, we also determine that the uncertainty in the future contribution of the Greenland Ice Sheet due to different climate forcings and the uncertainty due to the bed topography are comparable at the end of this century, however the uncertainty due to climate forcings dominates in the long run.

How to cite: Krishna, M., Morlighem, M., Mangini, D., and Choi, Y.: Quantifying the uncertainty in Greenland’s contribution to sea level rise due to the bed topography, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5996, https://doi.org/10.5194/egusphere-egu26-5996, 2026.

EGU26-6138 | ECS | Orals | CR2.4

Aq2 and Kq2, refined geothermal heat flow models from multivariate observables for application to ice sheet modelling 

Tobias Stål, Felicity S. McCormack, Anya M. Reading, and Magued Al-Aghbary and the Aq2 Interdisciplinary Research Collaboration

Geothermal heat plays an important role in basal ice sheet processes, potentially influencing the stability of Antarctica’s interior ice sheets. Modelled geothermal heat flow can yield discrepancies due to methodological choices and limited data. Recent advances in multivariate analysis and empirical methods have resolved many of these inconsistencies, yielding more consistent outputs that now serve as valuable inputs to ice sheet simulations. Nevertheless, substantial uncertainties remain, particularly in regions with sparse observational coverage. A key factor in addressing these challenges is the spatial resolution of heat flow maps, which governs how basal melt is represented in ice sheet dynamics.

 

We introduce two new geothermal heat flow models designed for glaciated regions: Aq2, developed for continental Antarctica, and Kq2, developed for Greenland. Both models utilise a common framework and employ a multivariate, empirical similarity approach that integrates 18 of the most recent and highest quality observables with the latest reference geothermal heat database, to which we apply weighting and pre-processing to improve representation. Compared to previous empirical models, Aq2 and Kq2 offer reduced uncertainty, greater robustness, and refined spatial resolution. Geothermal heat flow is mapped onto a 0.5 × 0.5 km grid using a forward redistribution approach, which enables higher spatial resolution by leveraging refined observations where available.

 

The models are openly shared in interoperable formats, complete with uncertainty estimates and reproducible code.

How to cite: Stål, T., McCormack, F. S., Reading, A. M., and Al-Aghbary, M. and the Aq2 Interdisciplinary Research Collaboration: Aq2 and Kq2, refined geothermal heat flow models from multivariate observables for application to ice sheet modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6138, https://doi.org/10.5194/egusphere-egu26-6138, 2026.

EGU26-6643 | ECS | Orals | CR2.4

Unravelling the importance of iceberg-calving-induced hydrodynamic forces to monitor Greenland ice mass loss with seismic inversion of glacial earthquakes 

Nicolas De Pinho Dias, Alban Leroyer, Justin C Burton, Wambui Ngugi, Andreas Kjær Dideriksen, Eugenio Ruiz-Castillo, William D. Harcourt, Jeffrey Taylor Kerby, Søren Rysgaard, Olivier Castelnau, and Anne Mangeney

Marine-terminating glaciers play a significant role he loss of ice mass from Greenland. Iceberg calvings are thought to account for about half of Greenland ice mass loss. These events produce seismic waves (glacial earthquakes) recorded by global seismic networks and contain information such as the iceberg volume and the forces acting during the event. Previous work showed that seismic inversion, coupled to numerical modeling, can be used to decipher the glacial earthquake signal [Sergeant 2019]. However, the lack of consideration for the hydrodynamic forces applied onto the glacier leads to large uncertainties in the iceberg volume estimations. Therefore, based on previous work, a Computational Fluid Dynamics (CFD) model is employed to model the complex fluid/structure interaction between a capsizing iceberg and the ocean. The simulations match results from laboratory experiments with great accuracy (rotation kinematics, effect of calving type, hydrodynamic pressure, etc.) [De Pinho Dias 2025].

In this presentation, we will show how the forces applied onto a simple model of Helheim glacier during an iceberg calving depend on geometrical parameters (iceberg height, aspect ratio, water depth, iceberg drop height). The pressure force exerted onto the glacier front has a significant magnitude of more than 50 % of the iceberg/glacier contact force which acts in the opposite direction.

The forces are then converted into seismic signals and show a very good match with the signal recorded at 8 stations in Greenland.

In addition, we will show the path of particle tracers advected by calving-induced water currents.

 

Sergeant, A. et al. (2019) ‘Monitoring Greenland ice sheet buoyancy-driven calving discharge using glacial earthquakes’, Annals of Glaciology, 60(79), pp. 75–95. doi:10.1017/aog.2019.7.

De Pinho Dias, N., Leroyer, A., Mangeney, A. and Castelnau, O., 2025. Fluid-structure modeling of iceberg capsize. Ocean Engineering, 336, p.121765. doi:10.1016/j.oceaneng.2025.121765

 

How to cite: De Pinho Dias, N., Leroyer, A., Burton, J. C., Ngugi, W., Dideriksen, A. K., Ruiz-Castillo, E., Harcourt, W. D., Kerby, J. T., Rysgaard, S., Castelnau, O., and Mangeney, A.: Unravelling the importance of iceberg-calving-induced hydrodynamic forces to monitor Greenland ice mass loss with seismic inversion of glacial earthquakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6643, https://doi.org/10.5194/egusphere-egu26-6643, 2026.

EGU26-7367 | Orals | CR2.4

age_flow_line-1.0: a fast and accurate numerical age model for a pseudo-steady flow tube of an ice sheet 

Frédéric Parrenin, Ailsa Chung, and Carlos Martín

Numerical age models are useful tools for investigating the age of the ice in an ice sheet. They can be used to date ice cores or to interpret isochronal horizons which are observed by radar instruments. Here, we present a new numerical age model for a flow line of an ice sheet. The assumption here is that the geometry of the flow line and the velocity shape functions are steady (i.e. constant in time). A time-varying factor can only be applied to the surface accumulation rates and basal melting rates. Our model uses an innovative logarithmic flux coordinate system (π , θ ), previously published, which is suitable for solving transport equations because it tracks ice trajectories. Using this coordinate system, solving the age equation is simple, fast and accurate, because the trajectories of ice particles pass exactly through the nodes of the grid. Our numerical scheme, called Eulerian-Lagrangian, therefore combines the advantages of Eulerian and Lagrangian schemes. We present an application of this model to the flow line going from Dome C to the Beyond EPICA Little Dome C drill site and show that horizontal flow is a non-negligible factor which should be considered when modelling the age-depth relationship of the Beyond EPICA ice core. The code we developed for age modelling along a flow tube is named age_flow_line-1.0 and is freely available under an open-source license.

How to cite: Parrenin, F., Chung, A., and Martín, C.: age_flow_line-1.0: a fast and accurate numerical age model for a pseudo-steady flow tube of an ice sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7367, https://doi.org/10.5194/egusphere-egu26-7367, 2026.

Among components of the cryosphere, the Greenland Ice Sheet (GrIS) is currently the largest contributor to global mean sea-level rise, driven by both enhanced surface melt and dynamic ice loss to the ocean. Evidence from the Holocene suggests that the GrIS can undergo substantial deglaciation under climatic conditions only slightly warmer than at present day. However, projections of its future evolution remain highly uncertain, largely due to the heterogeneous response of individual outlet glaciers to ocean forcing, particularly in the relatively understudied and sparsely sampled northern GrIS.

In this project, we investigate the present-day state and future evolution of the northern GrIS, with a specific focus on CH Ostenfeld Glacier. This glacier lost its floating extension completely decades ago, which could be a precursor of the fate of the nearby Ryder and Petermann glacier. We use the Ice-sheet and Sea-level System Model (ISSM) for this purpose. We integrate new ice-penetrating radar observations of the subglacial topography in the grounding zone of Ostenfeld Glacier, collected during the GEOEO 2024 North of Greenland Expedition aboard the ice breaker Oden. Together with existing subglacial topography datasets these data are used to assess the sensitivity of modelled glacier behaviour to variations in subglacial topography. Using the updated subglacial topography dataset, we furthermore investigate the subglacial hydrological network. Modelled freshwater fluxes from this network will be used to investigate the interaction between the marine-terminating ice sheet and fjord circulation, in collaboration with researchers from the Tracing How Atlantic Water Influences Northern Greenland (THAWING) project. This coupling governs the delivery of warm Atlantic Water to the glacier grounding zone and, consequently, the magnitude of frontal melt at CH Ostenfeld Glacier. The freshwater released from the CH Ostenfeld glacier through this frontal melting or from the subglacial hydrological network, will influence the fjord circulation and thereby the availability of Atlantic Water at the front of the glacier. 

How to cite: van den Akker, T., Wang, Z., and Kirchner, N.: Modelling of the present-day state and future evolution of CH Ostenfeld glacier, northern Greenland, using new subglacial topography observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7655, https://doi.org/10.5194/egusphere-egu26-7655, 2026.

EGU26-7880 | ECS | Posters on site | CR2.4

Modelling the evolution of the hydrothermal structure of polythermal glaciers in Svalbard 

Lucie Bacchin and Francisco Navarro

Svalbard is among the fastest warming regions on Earth, with mean air temperatures rising several times faster than the global average. Approximately 57% of the archipelago remains glacierized, and most of these glaciers are polythermal, containing both cold and temperate ice layers. Understanding their response to ongoing and future climate change requires physically-based thermomechanical modelling capable of capturing the evolution of internal ice temperatures and cold–temperate transitions.


In this study, we apply the Instructed Glacier Model (IGM), an open-source, Python-based glacier model that integrates climate-driven surface mass balance, ice-flow and heat transfer processes. IGM further employs physics-informed machine learning and GPU acceleration to efficiently resolve high-order ice-flow dynamics, enabling large-scale simulations at high spatial resolution.


Svalbard benefits from extensive ground-penetrating radar (GPR) datasets, providing rare observational constraints on the cold–temperate transition surface (CTS). We exploit multi-epoch GPR observations to evaluate the ability of IGM thermodynamics to reproduce the observed CTS evolution. As a first step in a broader PhD project aiming to simulate the evolution of all land-terminating Svalbard glaciers under different greenhouse gas emission scenarios, we focus on Werenskioldbreen, a well-instrumented glacier with repeated GPR surveys (1998, 2008, 2016, 2024) and long-term mass-balance records. This work provides a crucial benchmark for improving thermomechanical modelling of polythermal glaciers and contributes to reducing uncertainties in projections of Svalbard glacier change.

How to cite: Bacchin, L. and Navarro, F.: Modelling the evolution of the hydrothermal structure of polythermal glaciers in Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7880, https://doi.org/10.5194/egusphere-egu26-7880, 2026.

EGU26-8003 | ECS | Orals | CR2.4

Simulating the ice flow of marine ice sheets and outlet glaciers with IGM, a physics-informed deep-learning model 

Thomas Gregov, Sebastian Rosier, Brandon Finley, Andreas Vieli, and Guillaume Jouvet

Marine sectors of ice sheets and marine-terminating glaciers are pivotal to cryospheric mass loss. Despite their limited areal extent, marine regions strongly regulate ice discharge across the grounding line. Moreover, although most glaciers are not marine-terminating, those that are represent a large share of total glacier ice volume and, among glaciers, dominate the potential glacier contribution to future sea-level rise. Accurately representing marine regions in ice-flow models is thus essential.

Here, we present current progress towards extending IGM to account for marine regions. IGM is a model that uses physics-informed machine learning to simulate ice-flow dynamics (Jouvet and Cordonnier, 2023). In IGM, the mapping between glacier configuration (e.g., geometry) and ice velocity can be obtained either with classical numerical approaches or by learning a neural-network surrogate through the optimization of its weights. The model is implemented in Python with a modular design, which facilitates the implementation and modification of individual physical components, and enables the use of high-performance libraries such as TensorFlow for GPU computing. IGM has demonstrated orders-of-magnitude speedups over classical solvers and has enabled continental-scale, long-term simulations of mountain glaciers (e.g., Leger et al., 2025).

However, IGM was not originally developed for marine settings. Extending it to such regions is challenging because (i) the stress balance differs from that of grounded ice, with negligible basal friction, (ii) the resulting dynamics are markedly more nonlocal due to the stronger influence of membrane stresses (the elliptic terms in the stress balance), and (iii) the transition from grounded to floating ice occurs over short spatial scales, on the order of a few hundred meters. We describe the progress made to address these challenges, including a multiscale strategy that locally decouples distinct flow regimes. We will present results on idealized test cases, with particular attention to numerical accuracy and computational efficiency.

How to cite: Gregov, T., Rosier, S., Finley, B., Vieli, A., and Jouvet, G.: Simulating the ice flow of marine ice sheets and outlet glaciers with IGM, a physics-informed deep-learning model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8003, https://doi.org/10.5194/egusphere-egu26-8003, 2026.

EGU26-9268 | Posters on site | CR2.4

Modelling the surges of Vernagtferner (Ötztal Alps) since 1599 

Martin Rückamp and Christoph Mayer

The Vernagferner in the Ötztal Alps has a history of several surges since 1599. The occurrence was periodic, with a short active advance and a much longer retreat; the whole cycle lasted, on average, 82 years. The mode of ice flow typically changed, i.e., the surge speed increased by more than one order of magnitude with heavy crevassing. The dimensions of advance and retreat were much larger than those known from other glaciers in the area (Hoinkes 1969).

In general, the understanding of surging glaciers is limited due to the sheer diversity of surge-type glaciers. Consequently, numerous mechanisms have been proposed to explain glacier surging. Here, we follow the approach by Benn et al. (2019), which includes both temperate and polythermal glacier surges, based on a coupled ice-flow and enthalpy description. The theory parameterizes key thermodynamic and hydrological processes, including surface-to-bed drainage and distributed and channelized drainage systems. The lumped-element model is extended to realistic 3D geometries and implemented within the existing enthalpy framework of the Ice-sheet and Sea-level System Model. We illustrate the surging behaviour on a simplified 3D glacier geometry and present preliminary results of the Vernagtferner.

REFERENCES

Hoinkes, H. C. (1969): Surges of the Vernagtferner in the Ötztal Alps since 1599, Canadian Journal of Earth Sciences, Vol. 6, No. 4, p. 853-861

Benn, D. I., Fowler, A. C., Hewitt, I., Sevestre, H. (2019): A general theory of glacier surges, Journal of Glaciology, Vol. 65, No. 253, p. 701-716

How to cite: Rückamp, M. and Mayer, C.: Modelling the surges of Vernagtferner (Ötztal Alps) since 1599, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9268, https://doi.org/10.5194/egusphere-egu26-9268, 2026.

EGU26-9372 | ECS | Posters on site | CR2.4

Age field and particle trajectories using a 2.5D inverse model along a flowline from DF to EDML, Antarctica  

Ailsa Chung, Frédéric Parrenin, Olaf Eisen, and Daniel Steinhage

We present a 2.5D pseudo-steady state inverse model applied to the flow line from Dome Fuji (DF) to the EPICA Dronning Maud Land (EDML) ice core drill site. The model is constrained by radar horizons dated from 4-132 ka using the DF ice core chronology. We interpolate and extrapolate the age field using these horizons. The simplicity of our 2.5D numerical integration scheme results in an efficient computation time allowing us to use inverse methods to determine poorly known parameters such as surface accumulation rate, velocity profile and basal conditions.

We find that the amount of basal melting along the DF-EDML flowline generally correlates with higher ice thickness. We also look at the spatial origin of particles now at the EDML drill site, as this is an important consideration for corrections in measurements of the ice core itself. We compare to a Huybrechts et al. 2007 who used a more complex model on the same area. Finally, we look at areas along the flowline where ice >1Ma could potentially be found.

How to cite: Chung, A., Parrenin, F., Eisen, O., and Steinhage, D.: Age field and particle trajectories using a 2.5D inverse model along a flowline from DF to EDML, Antarctica , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9372, https://doi.org/10.5194/egusphere-egu26-9372, 2026.

EGU26-9524 | Posters on site | CR2.4

Towards a particle-based finite element framework for ice calving simulation 

Sayako Hirobe, Yota Sato, and Kenji Oguni

Calving of ice shelves and tidewater glaciers plays a critical role in controlling glacier and ice-sheet mass loss, yet its physical representation in numerical models remains challenging due to the strong coupling between continuum deformation, fracture initiation, and discrete separation processes. Direct observations of calving are limited by field accessibility and satellite temporal resolution, highlighting the need for numerical models to investigate calving mass loss and its mechanisms, and to explore future scenarios and sensitivity experiments. In this study, we present the preliminary development of a numerical framework for the analysis of calving-related mechanical processes based on a Particle Discretization Scheme Finite Element Method (PDS-FEM).

PDS-FEM is a numerical approach originally developed for quasi-static and dynamic fracture problems in solid mechanics, including fracture propagation in residual stress fields. The method provides a particle description to the solid continuum with a mathematically consistent finite element formulation. This particle discretization scheme enables precise evaluation of deformation, stress localization, and crack initiation without prescribing explicit crack paths or tuning parameters. In this initial phase, we focus on formulating the governing equations, implementing the numerical scheme, and examining its basic mechanical behavior under simplified conditions relevant to calving.

We investigate simplified three-dimensional configurations to examine the basic mechanical behavior of ice under tensile and bending stresses which are commonly associated with calving processes near ice fronts. Constitutive laws and boundary conditions are intentionally simplified, and therefore the results are qualitative and intended to demonstrate feasibility rather than provide quantitative predictions.

While the present results are preliminary, this work demonstrates the potential of PDS-FEM as a framework for analyzing calving which includes continuum ice dynamics and fracture-related processes. Future work will focus on model validation, applications to more realistic glacier and ice-shelf geometries, and exploring more complex constitutive laws for ice deformation.

How to cite: Hirobe, S., Sato, Y., and Oguni, K.: Towards a particle-based finite element framework for ice calving simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9524, https://doi.org/10.5194/egusphere-egu26-9524, 2026.

Geothermal Heat Flow (GHF) is an important and poorly constrained boundary condition on the grounded parts of the Antarctic ice sheet. Almost all existing estimates of Antarctic GHF are based on solid-earth observables such as magnetic anomalies or the seismic structure of the upper mantle. However, many glaciological observations are sensitive to the thermal structure of the ice sheet, such as subglacial lakes identified through both ice-penetrating radar and satellite altimetry, radar reflectivity and specularity, basal freeze-on, borehole temperature measurements, and more. Here, I present the first preliminary results from a project that aims to solve for Antarctic GHF by inverting an ice sheet thermal model to fit glaciological observations. This model is a 3D steady-state enthalpy-conserving advection-diffusion model for ice temperature, coupled to a balance-flux model of subglacial hydrology capable of producing both melt and basal freeze-on, along with a 3D balance ice flow and rheology model constrained by surface gradients and the observed flow direction. Forward model runs forced by a geophysically-informed GHF prior reveal a wealth of detail on the Antarctic thermal structure. In this model, West Antarctica is almost completely warm-based because of the high GHF prior there, while East Antarctica has a mixed thermal state. Fast-flowing ice streams are almost completely warm-based because of the influence of strain heating, suggesting they will have relatively limited sensitivity to GHF. Thick temperate layers (i.e., temperate ice above the basal plane) are rare overall but are present in roughly 25% by area of the fast-flowing ice streams, suggesting that they may play an important role in regulating the resistance to flow in dynamically important regions. To prepare for the inversion, I compile a wide range of glaciological observations, including assembling and leveling radar reflectivity data from many disparate campaigns and sources. I define a multi-part cost function using a variety of glaciological observations, rheological constraints, a geophysical prior, and a regularization term. I then derive a formulation for the adjoint of the 3D model that can be computed using the same solver as the forward model, allowing rapid computation of down-gradient step direction during the inversion. The computed adjoint reveals how information from observational constraints is transported upstream in both ice and water flow to constrain boundary conditions in the catchment above the observations. I test the computed adjoint using finite difference perturbations at a selection of representative regions and find good agreement, giving me confidence that it can be used to guide an inversion. I conclude by running a first test inversion, showing that the computed adjoint can indeed be used to tune GHF to fit observational constraints. The next steps include filling out the remaining observational constraints, especially with additional basal freeze-on data, and L-curve analysis to guide selection of the (currently arbitrary) regularization term.

How to cite: Wolovick, M.: 3D Thermal Modeling of Antarctica in Preparation for Heat Flow Inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9531, https://doi.org/10.5194/egusphere-egu26-9531, 2026.

EGU26-9750 | ECS | Orals | CR2.4

Modelling the evolution of Thwaites Glacier over the 20th century 

David Bett, Alexander Bradley, Bertie Miles, C Rosie Williams, Paul Holland, and Robert Arthern

Thwaites Glacier is rapidly evolving and could make large sea-level contributions in the coming centuries, making it essential to understand the drivers of the ongoing ice loss. Sediment core analysis suggests that Thwaites Glacier was in a relatively quasi-steady state for millennia before its western pinning point ungrounded in the 1940s. We use the MITgcm-WAVI coupled ocean-ice sheet model to create example quasi-steady pre-1940s configurations for Thwaites Glacier, including a most plausible pre-1940s state, finding that healing the damaged ice shelf is necessary to achieve this. Next, we trigger ice retreat and highlight key processes as the model evolves into the present-day configuration, including ice damage, pinning-point ungrounding driven by ocean melting, and ice piracy between eastern and western Thwaites Glacier. By conducting reversibility experiments during the retreat, we find that multiple quasi-steady ice-sheet states are possible under the same ocean forcing, demonstrating the importance of feedbacks and possible tipping points in the system. Either ice damage or increased ocean forcing can eliminate these quasi-steady states, prompting retreat, as observed today.

How to cite: Bett, D., Bradley, A., Miles, B., Williams, C. R., Holland, P., and Arthern, R.: Modelling the evolution of Thwaites Glacier over the 20th century, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9750, https://doi.org/10.5194/egusphere-egu26-9750, 2026.

EGU26-10260 | ECS | Posters on site | CR2.4

ODINN.jl: A new modular, hybrid, differentiable glacier model  

Jordi Bolibar, Facundo Sapienza, Alban Gossard, Mathieu le Séac'h, Lucille Gimenes, Vivek Gajadhar, Fabien Maussion, Ching-Yao Lai, Bert Wouters, and Fernando Pérez

The representation of glacier ice flow dynamics in glacier models in response to climate change, such as basal sliding or rheology, remains a critical challenge, particularly in integrating mechanistic models based on differential equations with the growing availability of observational data. Here, we present ODINN.jl, an open-source, modular framework for hybrid glacier modelling that combines scientific machine learning (SciML) with physical process-based approaches based on partial differential equations (PDEs). The framework is designed to facilitate both forward and inverse simulations of glacier evolution, enabling the assimilation of diverse datasets—such as ice thickness, surface velocities, and climate reanalyses—into a unified modelling ecosystem.

We have recently released ODINN.jl v1.0 after almost 5 years of work, providing a new architecture and stable API structured as an interconnected suite of Julia packages, each addressing specific tasks: Sleipnir.jl for data management, Muninn.jl for surface mass balance, Huginn.jl for ice flow dynamics, and ODINN.jl itself as the SciML interface for differentiation, optimisation, and hybrid modelling. This architecture allows users to easily customise model components, swap physical parametrisations, and integrate data-driven models (e.g., neural networks) to represent sub-grid processes or empirical laws. A key feature of this framework is its capacity to leverage automatic differentiation and adjoint methods to optimise model parameters, initial conditions, and statistical regressors. Parallelization is available for both forward simulations and advanced inverse methods, such as universal differential equations (UDEs), to explore poorly understood processes like basal sliding or calving. An early prototype of the model showed its potential to learn hidden laws in a noisy synthetic dataset, and with this new stable release we are now moving to large-scale applications using regional remote sensing and field observations such as high-resolution ice surface velocities and ice thickness. 

ODINN.jl is compatible with the Open Global Glacier Model (OGGM) ecosystem, enabling simulations for virtually any glacier worldwide using preprocessed datasets (e.g., RGI outlines, DEMs, climate reanalyses). This new modelling framework offers a reproducible, open-source solution to bridge the gap between physical understanding and data-driven discovery. Through modularity, scalability, and open-source collaborative approaches, ODINN.jl aims to explore both methodological advancements and large-scale applied modelling in glaciology. 

How to cite: Bolibar, J., Sapienza, F., Gossard, A., le Séac'h, M., Gimenes, L., Gajadhar, V., Maussion, F., Lai, C.-Y., Wouters, B., and Pérez, F.: ODINN.jl: A new modular, hybrid, differentiable glacier model , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10260, https://doi.org/10.5194/egusphere-egu26-10260, 2026.

EGU26-10708 | ECS | Orals | CR2.4

Decomposing Seasonal Ice-flow Variability in Western Greenland using Modelling and Observations 

Kuba Oniszk, Jessica Badgeley, Gong Cheng, William Colgan, and Shfaqat Abbas Khan

Outlet glaciers of the Greenland Ice Sheet typically undergo a seasonal cycle in ice flow, yet the magnitude and timing of peak annual velocities vary substantially among glacier systems, across years, and with distance away from the terminus. At tidewater glaciers, this variability reflects mainly the competing influences of surface meltwater-driven basal lubrication and flexural perturbations associated with calving-front dynamics. Because observations alone cannot readily separate these processes, we develop a physics-based framework that integrates ice-flow simulations with high-resolution surface velocity observations to decompose seasonal ice motion into basal and frontal components.

We apply this approach to 61 tidewater glacier basins in western Greenland and show that seasonal velocity variations are primarily controlled by evolving basal hydrologic conditions. Frontal perturbations nonetheless exert a secondary but persistent influence on seasonal ice flow. Near glacier termini, mixed basal–frontal control occurs 49.6–62.3% of the time, and although the influence of frontal forcing generally diminishes inland, it can extend to elevations of up to 2000 metres above sea level at fast-flowing glaciers such as Sermeq Kujalleq (Jakobshavn Isbræ). Our method further isolates signals that are subdued in raw velocity observations and closer aligned with expected patterns of seasonal basal drainage development. Importantly, results from three independent transient model configurations demonstrate that our conclusions are robust to the choice of sliding law, with consistent identification of the dominant controlling process in 97.1% of cases. We therefore propose that this framework provides a reliable basis for process-level interpretation of seasonal ice-flow variability across Greenland.

How to cite: Oniszk, K., Badgeley, J., Cheng, G., Colgan, W., and Khan, S. A.: Decomposing Seasonal Ice-flow Variability in Western Greenland using Modelling and Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10708, https://doi.org/10.5194/egusphere-egu26-10708, 2026.

EGU26-11418 | ECS | Orals | CR2.4

Comparing methods of computing second order derivatives in numerical ice sheet models 

Trystan Surawy-Stepney and Steph Cornford

Large-scale continuum ice sheet models solve a set of conservation-of-momentum equations to calculate ice speed given the ice sheet geometry and, often, some a priori unknown parameters. To facilitate the initialisation of projections, many such models allow one to calcuate gradients of model outputs with respect to those unknown input paramters. In some models, this is done with the help of algorithmic differentiation (AD), while in others it is done using hand-derived PDE-level adjoint rules. Increasingly, there is interest in computing higher-order derivatives, for example, to facilitate the use of different optimisation algorithms or perform uncertainty quantification. In this work, we derive and implement a second-order adjoint (SOA) model for the shallow stream equations, implementable in any 2D ice sheet model. We implement this in a finite volume code written in a numerical computation library for Python called JAX. We conduct comparisons between the computation of Hessians using this SOA model and using the AD tools provided by JAX. The SOA model makes the assumption of linear rheology, as many first-order adjoint models do. We find that this causes a rapid departure in the directions of the principal components of the Hessian from those founding using AD. Hence, we consider AD to be the more suitable choice for many applications.

How to cite: Surawy-Stepney, T. and Cornford, S.: Comparing methods of computing second order derivatives in numerical ice sheet models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11418, https://doi.org/10.5194/egusphere-egu26-11418, 2026.

EGU26-11622 | ECS | Posters on site | CR2.4

Geothermal heat flow fields for ISMIP7 – Community recommendations for Antarctica & Greenland 

Mareen Lösing, William Colgan, Helene Seroussi, Tobias Stål, Tong Zhang, Felicity McCormack, Jörg Ebbing, Leigh Stearns, Anne Gravsholt Busck, Dominik Fahrner, Synne Høyer Svendsen, and Anya Reading

Geothermal heat flow (GHF) plays a fundamental role in regulating basal thermal conditions of ice sheets, influencing basal sliding, internal deformation, and lithospheric rheology. Despite its importance, GHF in polar regions remains poorly constrained due to the scarcity of borehole measurements and substantial divergence among existing geophysical and glaciological estimates. These discrepancies stem from differences in methodology, data availability, and underlying assumptions, leading many ice sheet models to rely on spatially uniform values, ensemble means, or legacy products that inadequately represent spatial variability. We review all available continent-wide GHF fields, analysing their methodologies and data sources, and provide recommendations on their use. GHF fields generally fall into three categories: (1) outdated due to improved data availability, (2) overly simplified parametrization, and (3) preferred fields. To further assess applicability, we conducted an online expert elicitation survey to identify the most suitable fields for ice sheet modeling, particularly for ISMIP7. For preferred fields, we discuss uncertainty and data dependency to guide their use in different applications.

In Antarctica, all fields agree on the broad division between low heat flow in East and higher heat flow in West Antarctica, though spatial patterns vary. Preferred fields serve as a baseline for local studies, which can incorporate additional datasets like magnetic depth estimates or regional geological constraints. In Greenland, uncertainty is particularly high at NGRIP, where estimation and observations are difficult to reconcile. Local heterogeneity impacts heat flow observations in ways that regional fields cannot yet fully address. Nonetheless, recent estimates suggest low to moderate heat flow under the Greenland ice sheet, indicating that the Iceland hot spot has a limited impact, while subglacial geology plays a dominant role in controlling local variations.

Results from the expert survey indicate broad support for multivariate, data-driven approaches that integrate geological and geophysical constraints, including recent fields by Stål et al. (2021), Lösing & Ebbing (2021), and Colgan et al. (2022). These methods are generally regarded as better equipped to use all existing information, represent spatial heterogeneity, provide uncertainty information, and remain consistent with inferred basal conditions. Importantly, the survey captures, as objectively as possible, the reasons why a given GHF field is a good choice as a representation to be used for ice sheet modelling, and hence, model intercomparisons.

Continued progress in GHF estimation will require both methodological innovation and improved data coverage. Integrating machine learning with physics-based models, fostering cross-disciplinary data integration, and increasing spatial resolution are key priorities. In the context of ISMIP7, we recommend moving beyond outdated or purely interpolated GHF products and adopting modern, data-driven fields that better reflect current understanding.

How to cite: Lösing, M., Colgan, W., Seroussi, H., Stål, T., Zhang, T., McCormack, F., Ebbing, J., Stearns, L., Gravsholt Busck, A., Fahrner, D., Høyer Svendsen, S., and Reading, A.: Geothermal heat flow fields for ISMIP7 – Community recommendations for Antarctica & Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11622, https://doi.org/10.5194/egusphere-egu26-11622, 2026.

EGU26-11796 | ECS | Orals | CR2.4

Incorporating Tidal Forcing into Long-Term Ice-Sheet Dynamics via Temporal Averaging 

Celine Reddig and Thomas Richter

Long-term models for ice-sheets and glaciers are in general modeled as very slow, viscous fluids, which allows for large time steps on the order of years. However, over the past few decades, observations and theoretical studies have shown that ice streams exhibit short-term responses when it comes to external forcing due to ocean tides, which induce for example non-linear velocity variations.

Short-term models typically apply viscous-elastic ice rheologies to capture these effects. However, resolving tidal dynamics requires very small time steps on the order of minutes, making long-term simulations computationally challenging.

To address this, we propose a temporal averaging approach to include short-term tidal effects into efficient, long-term simulations. We present initial results based on a two-component modeling framework. The long-term component models the ice sheet as a viscous fluid governed by the p-Stokes equations with free surfaces. The short-term component describes the elastic response of the ice to tidal forcing, modeled by an elasticity problem driven by variations in hydro-static pressure due to ocean tides. This leads to a variational inequality of Signorini type, reflecting intermittent contact between the ice and the bedrock. 

As the tidal cycle causes the ice–bedrock contact zone to evolve in time, the basal boundary condition alternates between frictional contact and floating due to ocean-pressure. By exploiting the periodic nature of the tidal forcing, we derive effective, tidally averaged basal traction coefficients based on the varying grounding line position. These effective coefficients can be incorporated into the basal friction law of the viscous, long-term ice-flow model. The averaged friction coefficients are updated after a time step in the long-term model to take the geometric deformation of the ice sheet into account. 

This approach allows for efficient simulations that capture the influence of short-term tidal dynamics on ice-streams effectively, and relies on a clear separation between the short tidal time scale and the long-term viscous dynamics of the ice sheet.

How to cite: Reddig, C. and Richter, T.: Incorporating Tidal Forcing into Long-Term Ice-Sheet Dynamics via Temporal Averaging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11796, https://doi.org/10.5194/egusphere-egu26-11796, 2026.

EGU26-12144 | ECS | Posters on site | CR2.4

Under what conditions will the Wilkes Subglacial Basin exhibit large scale retreat? 

Deborah Rhee, Sainan Sun, and Hilmar Gudmundsson
The Wilkes Subglacial Basin (WSB) holds approximately 3-4 m sea-level equivalent ice volume (Rignot et al., 2019; Crotti et al., 2022), and is characterised by a reverse-sloping bed, making it vulnerable to marine ice sheet instability. However, the conditions and indeed the possibility of large retreat is still highly debated. Using the finite element ice-sheet model, Úa, we conduct a sensitivity analysis to determine the climate conditions for large scale retreat. We further explored uncertainties arising from poorly known physical mechanisms, particularly the sliding law.
 
Our simulations are initialised using present-day ice dynamics reproduced through inversion methods. Transient simulations of 500 years are then conducted with different surface temperature forcing. In the control experiment, constant present-day thermal forcing is applied to the local quadratic parameterisation (Jourdain et al., 2020) for sub-ice-shelf melting, and surface mass balance is prescribed using constant RACMO model output (Noël et al., 2023). Increase of surface temperature proportionally increase precipitation and thermal forcing. A mesh convergence study with mesh sizes up to sub-kilometre scale is conducted to ensure our conclusions are numerically robust.
 
We increase the surface temperature by up to 8 degrees and the ocean temperature by up to 40 degrees with a range of different sliding laws. The migration of the grounding line positions, total ice volume and volume above floatation are calculated in order to determine if and where large scale retreat has occurred.

How to cite: Rhee, D., Sun, S., and Gudmundsson, H.: Under what conditions will the Wilkes Subglacial Basin exhibit large scale retreat?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12144, https://doi.org/10.5194/egusphere-egu26-12144, 2026.

EGU26-12663 | ECS | Orals | CR2.4

The impact of the friction law on coupled ice flow/subglacial hydrology modeling 

Koi McArthur, Christine Dow, and Shivani Ehrenfeucht

Basal sliding is a key component of ice motion that is implemented in ice flow models via the use of a friction law, a relation between the basal shear stress, basal sliding velocity, and the effective pressure. Recent studies have performed two-way coupling between two-dimensional subglacial hydrology models with inefficient and efficient drainage components, and ice flow models via the effective pressure in the friction law. However, to date, there has not been an investigation of the impact of the friction law on two-way coupled ice flow/subglacial hydrology modeling. Here, we examine the effect of the Budd friction law, the Schoof friction law, and two regularized-Coulomb friction laws that we develop, on coupled modeling in the Siple Coast of West Antarctica. We found that when using the Budd friction law, the basal shear stress failed to respond to changes in both ice speed and effective pressure in a fashion that was consistent with the state of the subglacial hydrologic system, and the Schoof friction law did not accurately estimate the state of the subglacial hydrologic system. Consequently, using the Budd and Schoof friction laws led to instabilities in ice motion and flooding of the subglacial hydrologic system due to dynamic thinning of ice. The new friction laws we developed ensured an accurate estimation of the state of the subglacial hydrologic system, and no such instabilities arose in the corresponding simulations.

How to cite: McArthur, K., Dow, C., and Ehrenfeucht, S.: The impact of the friction law on coupled ice flow/subglacial hydrology modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12663, https://doi.org/10.5194/egusphere-egu26-12663, 2026.

EGU26-12979 | Posters on site | CR2.4

Evolution of ice-shelf damage at Pine Island Ice Shelf using Elmer/ice and multiple satellite derived observations 

Romain Millan, Lucie Bacchin, Cyrille Mosbeux, Lucille Gimenes, and Kaian Shahateet

The stability of the Antarctic Ice Sheet is a key control on global sea-level rise, with ice shelves acting as critical regulators of glacier discharge into the ocean. Understanding the processes governing ice-shelf stability and glacier dynamics is therefore essential for improving projections of future sea-level change. Pine Island Glacier is among the most rapidly changing glaciers on Earth and plays a major role in Antarctic mass loss, currently ranking as the largest single contributor to Antarctic-driven global mean sea-level rise. Between 1992 and 2011, the Pine Island grounding line retreated by approximately 31 km, leading to a substantial increase in ice discharge. This dynamic evolution has been accompanied by weakening of shear margins and increased ice damage, expressed by the proliferation of crevasses and rifts, which reduces the glacier's ability to transmit resistive stresses. In this study, we simulate the evolution of damage in the Pine Island Ice Shelf using the Elmer/Ice finite-element model. We invert for ice viscosity and the related ice damage under the shallow shelf approximation. We investigate the sensitivity of modeled damage to different ice-thickness datasets derived from radar and laser altimetry as well as satellite photogrammetry, all constrained by the same surface velocity observations. We further assess the impact of dataset spatial resolution on the inferred damage fields and compare the results with fracture maps derived using deep learning on satellite imagery. To evaluate temporal changes, we perform a serie of inversions spanning 1992–2022, using time-evolving observations of surface velocity and ice-shelf thickness. Finally, we compare the evolution of ice-shelf damage with changes in the ice-shelf buttressing index to assess the overall influence of damage on the stability of Pine Island Glacier over the past decades. This study was funded as part of the ERC-research project IceDaM.

How to cite: Millan, R., Bacchin, L., Mosbeux, C., Gimenes, L., and Shahateet, K.: Evolution of ice-shelf damage at Pine Island Ice Shelf using Elmer/ice and multiple satellite derived observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12979, https://doi.org/10.5194/egusphere-egu26-12979, 2026.

EGU26-13396 | Posters on site | CR2.4

Thwaites Glacier loses ice even without ocean melting  

C Rosie Williams, Matt Trevers, Sainan Sun, Paul Holland, David Bett, Robert Arthern, and Alexander Bradley

Pine Island (PIG) and Thwaites (TG) glaciers currently dominate Antarctica's sea-level contribution. These glaciers began a synchronous retreat in the mid twentieth century when PIG ungrounded from a submarine ridge and Thwaites from its Western pinning point. The historical ice loss in this sector is ultimately caused by changes in ocean melting. However, it remains unclear the extent to which the ongoing ice loss is driven by anomalously warm present-day ocean conditions, potentially caused by anthropogenic climate change, or is an ongoing response to a natural climate anomaly in the 1940s, to which the ice sheet is still adjusting. Here, we probe these drivers of ice loss by completely removing the ocean forcing. We use three state-of-the-art ice sheet models to simulate the response of PIG and TG in an extreme hypothetical scenario of zero ocean melting, maintained over a policy-relevant timescale (150 years). We find that PIG thickens and re-advances to the prominent sea-bed ridge on which it was grounded prior to the 1940s. In contrast, Thwaites continues to lose ice (at a decreasing rate) over the next 150 years, despite the absence of sub-ice shelf melt. This tells us two things. Firstly, since all the forcing is removed in these experiments, the ice loss from Thwaites must have a substantial component that is an ongoing transient response to historical forcing. Secondly, the historical retreat of Thwaites has led to a present-day state that cannot re-advance under any ocean cooling measures. Thus, Thwaites is now in a dynamically different state to its 1940s configuration. While this does not imply commitment to irreversible future retreat, the historical mass loss from Thwaites is now built-in and cannot be reversed through reductions in ocean forcing alone. This further suggests that some future sea-level contribution is unavoidable on centennial timescales, even under strong policy interventions that result in ocean cooling.

How to cite: Williams, C. R., Trevers, M., Sun, S., Holland, P., Bett, D., Arthern, R., and Bradley, A.: Thwaites Glacier loses ice even without ocean melting , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13396, https://doi.org/10.5194/egusphere-egu26-13396, 2026.

EGU26-13628 | Posters on site | CR2.4

How sensitive is Thwaites glacier to ocean conditions? 

G. Hilmar Gudmundsson, Jan De Rydt, Daniel Goldberg, Mathieu Morlighem, and Benjamin Getraer
In its present geometric configuration, the Thwaites Ice Shelf exerts only a limited influence on the upstream dynamics of Thwaites Glacier. Previous studies have demonstrated that ice flux across the grounding line is largely insensitive to the presence or absence of the ice shelf. However, these assessments have predominantly relied on diagnostic stress‑balance modelling using the contemporary geometry. In this study, we extend that analysis by evaluating the role—if any—of ocean‑induced basal melting in shaping the near‑future (decadal‑scale) evolution of Thwaites Glacier. First, we systematically quantify the sensitivity of upstream ice‑flow velocities to changes in ice rheology and ice‑shelf thickness across a suite of geometries generated through transient ice‑flow simulations. Second, we incorporate new coupled transient ice–ocean simulations to examine how varying ocean conditions influence projected glacier evolution within this integrated modelling framework. Our results indicate that both the current state and near‑term evolution of Thwaites Glacier are largely decoupled from oceanic forcing. This finding reinforces the view that present‑day mass loss from Thwaites Glacier is not primarily driven by ocean conditions and that this situation is unlikely to change in the foreseeable future.
 

How to cite: Gudmundsson, G. H., De Rydt, J., Goldberg, D., Morlighem, M., and Getraer, B.: How sensitive is Thwaites glacier to ocean conditions?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13628, https://doi.org/10.5194/egusphere-egu26-13628, 2026.

EGU26-13787 | ECS | Posters on site | CR2.4

Systematic comparison of calving rate parametrisations in an ice-sheet dynamical simulation of the Antarctic Ice Sheet 

Tanja Schlemm, Ann Kristin Klose, and Torsten Albrecht

In recent years, a number of calving parametrisations have been derived and evaluated in simulations on the scale of individual glaciers. However, these new calving parametrisations have not yet been systematically tested in a continental-scale simulation of an ice sheet. We consider four rate-based calving parametrisations of which two match current observations from calving glaciers in Alaska (Mercenier et al. 2018) and the Antarctic Peninsula (Parsons et al. 2025), while the other two are designed as cliff calving parametrisations (Schlemm & Levermann 2019, Crawford et al. 2021) and give non-zero calving rates only for cliff heights larger than currently observed in calving glaciers.
We evaluate these calving parametrisations in an ice-sheet dynamical simulation of the Antarctic ice sheet using the Parallel Ice Sheet Model (PISM). Starting from an ISMIP6 present-day initial state at 8 km resolution, we apply each parametrisation under SSP5-8.5 forcing.
Already at the beginning of the simulation, when forcing is still similar to present day, parametrisations that match observations from current calving glaciers in Alaska and the Antarctic Peninsula produce spurious terminus retreat at locations where no retreat is observed so far. This is due to high initial cliff heights (>100m) along the coast in the ISMIP6 initial state.
In contrast, cliff calving laws, which include a critical cliff height threshold (below which no calving occurs) and produce smaller calving rates, are more conservative and better suited for continental-scale applications, despite not matching observations from current glaciers. However, even these more conservative laws can produce calving in locations where it's not expected. Better results are achieved, when calving of grounded ice is restricted to the Amundsen, Amery, Ross and Ronne-Filchner basins.

How to cite: Schlemm, T., Klose, A. K., and Albrecht, T.: Systematic comparison of calving rate parametrisations in an ice-sheet dynamical simulation of the Antarctic Ice Sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13787, https://doi.org/10.5194/egusphere-egu26-13787, 2026.

EGU26-14559 | ECS | Posters on site | CR2.4

Reconstructing Jakobshavn Isbræ's evolution from 1958 to 2025 with ISSM constrained by multi-mission observations 

Sina Marie Felten, Gong Cheng, Shfaqat Abbas Khan, and Mathieu Morlighem

Over the past decade, Greenland’s major outlet glaciers have more than doubled their contribution to global sea-level rise. Among these, Jakobshavn Isbræ, located in West Greenland, is the largest outlet glacier by drainage area, accounting for approximately 6.5% of the Greenland Ice Sheet. The pronounced acceleration of Jakobshavn Isbræ around 2000 has been widely attributed to the collapse of a substantial portion of its floating ice tongue and the retreat of its terminus. This collapse is thought to be linked to enhanced basal melting beneath the ice shelf, driven by the intrusion of warm ocean waters, as well as the increased calving activity associated with a reduction in sea ice within the fjord. Estimates of the rate of retreat and mass loss from 1950 to 2000 remain very uncertain due to the sparsity of data throughout that timeframe.
In this study, we develop a new high-resolution model of the region that is constrained by available observations to reconstruct the retreat, acceleration, and thinning of the glacier during this time period. We use Ice-sheet and Sea-level System Model (ISSM) to simulate Jakobshavn Isbræ from 1958 to 2025. Our analysis integrates a comprehensive set of observational data, including ice front positions derived from Landsat imagery, ice velocity variations, and surface elevation changes. The simulations are performed on an unstructured, adaptively refined mesh with a model resolution reaching 100 m within the first few kilometers around the terminus position. The resulting transient simulations document the temporal evolution of glacier mass balance from 1958 to the present. Model performance is evaluated by comparing simulated ice volume changes with independent volume estimates derived from CryoSat-2, Envisat,  ICESat, ICESat-2, and NASA’s Operation IceBridge Airborne Topographic Mapper, as well as digital elevation models from 1964 and 1985, providing a robust reconstruction of Jakobshavn's recent history.

How to cite: Felten, S. M., Cheng, G., Khan, S. A., and Morlighem, M.: Reconstructing Jakobshavn Isbræ's evolution from 1958 to 2025 with ISSM constrained by multi-mission observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14559, https://doi.org/10.5194/egusphere-egu26-14559, 2026.

EGU26-14627 | Posters on site | CR2.4

Initialization and Projection of the Greenland Ice Sheet with the PoLarIS model 

Tong Zhang and Wei Leng

This study presents the application of the Polar Land Ice Simulator (PoLarIS) to initialize and project the dynamics of the Greenland Ice Sheet (GrIS). Accurately simulating the GrIS is critical for predicting its contribution to sea-level rise, yet challenges persist in representing its present-day state and future evolution. The initialization of the PoLarIS model leverages advanced data assimilation techniques, integrating high-resolution satellite and airborne observations to constrain the initial ice geometry, velocity, and basal conditions, thereby reducing discrepancies with the observed present-day ice sheet configuration. For projecting future dynamics, the model incorporates key physical processes, including thermomechanical coupling and evolving basal conditions, to simulate ice flow and mass balance under different climatic scenarios. The simulations highlight the significant role of marine-terminating outlet glaciers and the sensitivity of the ice sheet to oceanic and atmospheric forcings. Results underscore the importance of accurate initialisation for reliable centennial-scale projections and demonstrate the PoLarIS model's capability in contributing to improved estimates of the GrIS's future mass loss

How to cite: Zhang, T. and Leng, W.: Initialization and Projection of the Greenland Ice Sheet with the PoLarIS model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14627, https://doi.org/10.5194/egusphere-egu26-14627, 2026.

EGU26-14739 | Orals | CR2.4

Rheological control of crystal fabrics on Antarctic ice shelves 

Nicholas Rathmann, David A. Lilien, Daniel H. Richards, Felicity S. McCormack, and Maurine Montagnat

Ice crystal fabrics can exert significant rheological control on ice sheets and ice shelves, potentially softening or hardening anisotropic ice by several orders of magnitude compared to isotropic ice. We introduce an anisotropic extension of the Shallow Shelf Approximation (SSA), allowing for fabric-induced viscous anisotropy to affect the flow of ice shelves in coupled, transient simulations. We show that the viscous anisotropy of synthetic ice shelves can be parameterized using an isotropic flow enhancement factor, suggesting that existing SSA flow models could, with little effort, approximate the effect of fabric on flow. Next, we propose a new way to directly solve for SSA fabric fields using satellite-derived velocities, assuming velocities are approximately steady and that fabric evolution is dominated by lattice rotation with or without discontinuous dynamic recrystallization. We apply our method to the Ross and Pine Island ice shelves, Antarctica, suggesting that these regions might experience significant fabric-induced hardening and softening depending on the relative strength of lattice rotation and recrystallization. Our results emphasize the icedynamical relevance of needing to better constrain the strength of fabric processes. This calls for more widespread fabric and temperature measurements from the field, since measurements are currently too sparse for model validation.

How to cite: Rathmann, N., A. Lilien, D., H. Richards, D., S. McCormack, F., and Montagnat, M.: Rheological control of crystal fabrics on Antarctic ice shelves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14739, https://doi.org/10.5194/egusphere-egu26-14739, 2026.

EGU26-14757 | Orals | CR2.4

Modelling the transition in ice-dynamics from land- to lake-terminating glaciers: a case study in Iceland  

Jaime Otero, Daniel Goldberg, Peter Nienow, and Yefan Wang

Glaciers interact with adjacent proglacial lakes through a range of thermomechanical processes. These interactions occur in addition to climate-driven ablation but are capable of amplifying or modifying climatic effects through various feedback mechanisms. In particular, the connection between lake water-level and the subglacial hydrological system can reduce basal friction, which in turn leads to increased glacier flow and dynamic thinning. This creates a positive feedback loop in which decreased effective pressure, also driven potentially by negative surface mass balance, enhances flow velocity, in line with similar processes observed at marine-terminating glaciers.

Our aim in this study is to develop a simple model that can be used to understand the critical controls on the dynamic behaviour of glaciers as they transition from land- to lake-terminating systems. Here, we investigate the behaviour of Skaftafellsjökull in Iceland, which has undergone such a transition over the past twenty-five years. More specifically, we use the Shallow Shelf Approximation (SSA) in Elmer Ice to model ice dynamics, incorporating a water pressure-dependant friction law to model basal sliding with a simple parameterization of basal water pressure.

The model successfully reproduces the observed velocity patterns, capturing the shift from deceleration near the front in 2010 to pronounced acceleration in 2018–2020, reflecting the growing influence of the proglacial lake. We find a threshold behaviour between basal water pressure and ice velocity, whereby small increases in water pressure beyond a critical value led to strong acceleration, consistent with previous empirical observations. Furthermore, our results imply that surface thinning exerts a stronger control on the near terminus acceleration than the observed terminus retreat.  Our results suggest that the modelling framework developed provides a valuable tool for simulating these complex interactions in a computationally efficient manner.

How to cite: Otero, J., Goldberg, D., Nienow, P., and Wang, Y.: Modelling the transition in ice-dynamics from land- to lake-terminating glaciers: a case study in Iceland , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14757, https://doi.org/10.5194/egusphere-egu26-14757, 2026.

EGU26-15140 | Orals | CR2.4

The current and future state of subglacial hydrology and ice dynamics model coupling. 

Christine Dow, Shivani Ehrenfeucht, Koi McArthur, Mathieu Morlighem, and Felicity McCormack

Ice dynamics plays a primary role in rapid sea level rise, and our approach to ice dynamic modeling therefore determines our ability to assess future ice mass changes and resulting global implications. Over the last several years, the coupling of subglacial hydrology and ice dynamics models has allowed an enhanced analysis of the impact of basal boundary conditions and drainage networks on ice flux. Here, we discuss the progress to date of hydrology-ice dynamics coupling within the Ice-sheet and Sea-level System Model (ISSM), the impacts from coupling on hydrology and ice dynamic development, and the challenges that remain to better represent the ice-bed system in both catchment and continent-scale simulations. We also examine the role of projected surface melt in Antarctica and how that may affect subglacial hydrology development, basal sliding, and ocean melt under floating ice shelves. We outline the next steps for the field of hydrology-ice dynamics coupling and how this can benefit the wider glaciological community.

How to cite: Dow, C., Ehrenfeucht, S., McArthur, K., Morlighem, M., and McCormack, F.: The current and future state of subglacial hydrology and ice dynamics model coupling., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15140, https://doi.org/10.5194/egusphere-egu26-15140, 2026.

EGU26-16669 | Posters on site | CR2.4

Discussions on the ISMIP7 Antarctic ice-ocean forcing protocol 

Ronja Reese, Nicolas Jourdain, Xylar Asay-Davis, Erwin Lambert, Clara Burgard, Yoshihiro Nakayama, Tore Hattermann, Qin Zhou, Shenjie Zhou, Paul Holland, Pierre Dutrieux, and Sophie Nowicki

In past decades, substantial advances on understanding ocean–ice-shelf interactions have been made, and a number of parameterisations that provide sub-shelf melting for ice sheet modelling studies have been developed. Through ISMIP6, it was found that the choice of parameter values in melt parameterisations can influence the order of magnitude of melt rate changes in projections. Moreover, it has been shown that constraining those parameters with present-day observations is not sufficient to constrain melt rate changes under future warming. For ISMIP7, we hence propose a “come-as-you-are” approach for the choice of the sub-shelf melt parameterisation, but suggest a protocol for calibrating parameters using ocean model simulations and observations that show large changes in cavity temperatures as additional constraints. This is embedded into an updated and revised protocol for processing CMIP model data for the ISMIP7 Antarctic ice-ocean forcing protocol.

Come to the presentation if you are interested to learn (more) about the protocol, discuss your testing experiences, or provide feedback.

How to cite: Reese, R., Jourdain, N., Asay-Davis, X., Lambert, E., Burgard, C., Nakayama, Y., Hattermann, T., Zhou, Q., Zhou, S., Holland, P., Dutrieux, P., and Nowicki, S.: Discussions on the ISMIP7 Antarctic ice-ocean forcing protocol, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16669, https://doi.org/10.5194/egusphere-egu26-16669, 2026.

EGU26-17396 | ECS | Posters on site | CR2.4

Grounding-Line-Centred Diagnostics of Ice Discharge in the Amundsen Sea Sector 

Marine de Coatpont, Cyrille Mosbeux, and Gaël Durand

The accelerating rate of global sea-level rise underscores the growing importance of
understanding how ice sheets respond to climate forcing and how this response is
represented in models. The Antarctic Ice Sheet (AIS) represents one of the largest potential
contributors to future sea-level rise, yet its projected contribution remains highly uncertain,
reflecting limitations in our understanding and representation of key dynamical processes.
Improving confidence in future projections therefore requires a clearer assessment of ice-
sheet model behaviour and of the mechanisms that control ice discharge, particularly in
dynamically active regions. To this end, we analyse ensemble simulations from ISMIP6,
which provide a unique framework to explore the diversity and consistency of ice-sheet
model responses under common climate forcings. Unlike most analyses, which evaluate
model evolution over time, here we focus on the Amundsen Sea sector and compare the
local response of models when a grid point corresponds to the grounding line. This
grounding-line-centred diagnostic allows us to assess how ice flux, thickness, and velocity
vary as the grounding line migrates, and to explore the consistency of these relationships
across models. By focusing on local dynamical behaviour rather than time-integrated
evolution, this approach aims to improve our understanding of how grounding-line
processes control ice discharge in a region that dominates Antarctic mass loss.

How to cite: de Coatpont, M., Mosbeux, C., and Durand, G.: Grounding-Line-Centred Diagnostics of Ice Discharge in the Amundsen Sea Sector, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17396, https://doi.org/10.5194/egusphere-egu26-17396, 2026.

EGU26-18793 | ECS | Posters on site | CR2.4

Basal environment uncertainty and the triggering of Antarctic Ice Sheet tipping points 

Shivani Ehrenfeucht, Torsten Albrecht, Ann Kristin Klose, Donovan Dennis, and Ricarda Winkelmann

Recent studies show that critical thresholds, tipping points, likely exist for the Antarctic Ice Sheet, and potentially individual drainage basins within Antarctica. Surpassing these critical thresholds for key glacier drainage basins can have significant impacts on the long-term sea-level contribution of the ice sheet, which may be irreversible. The marine ice sheet instability (MISI) is considered to be one of the key feedback mechanisms capable of triggering tipping dynamics in ice sheets, wherein grounding line retreat past a stable position along the bed can trigger further rapid and extensive retreat due to the internal dynamics of ice flow. Model simulations that exhibit this instability tend to project much higher degrees of sea-level rise than those where MISI is not initiated. As such, it is important to understand what factors determine if MISI takes effect and the timing of its onset. The sliding velocity of a glacier is a fundamental variable in calculating overall ice flow, and how the sliding velocity evolves in time is a critical factor in determining if MISI is triggered or not during model simulations projecting future glacier dynamics. While it is well understood that the sliding velocity is highly dependent upon the basal environment, much remains unknown regarding its specific characteristics including where sediment accumulates and how much is present, how meltwater flows through the basal environment, and how to best represent basal friction felt by the glacier. Uncertainties associated with both the physical processes governing ice sheet responses to climate warming, and the parameter choices associated with those physical processes make the analysis of potential ice sheet tipping points particularly difficult. Here, we aim to better understand the influence that the basal environment has on the tipping behavior of the Antarctic Ice Sheet. We use the Parallel Ice Sheet Model (PISM) to identify critical temperature thresholds that will lead to irreversible ice sheet mass loss and quantify the associated long-term sea-level commitment from Antarctica. Climate forcings will be dictated according to the TIPMIP protocols, following stylized warming scenarios and exploring the ice sheet equilibrium response to constant climates at different global warming levels. We analyze model results for differences in tipping behavior obtained by using various different representations of hydrology in the basal environment and ranging values for associated parameters. Here, we present the initial results of these experiments and discuss the relative importance of subglacial hydrology in determining if and when critical tipping points are exceeded for the Antarctic Ice Sheet. 

How to cite: Ehrenfeucht, S., Albrecht, T., Klose, A. K., Dennis, D., and Winkelmann, R.: Basal environment uncertainty and the triggering of Antarctic Ice Sheet tipping points, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18793, https://doi.org/10.5194/egusphere-egu26-18793, 2026.

EGU26-18806 | ECS | Posters on site | CR2.4

Till calving do us apart: Systematising data assimilation of frontal ice retreat for glacier evolution modelling of marine- and lake-terminating glaciers 

Veena Prasad, Oskar Herrmann, Mamta K. c, Alexander R. Groos, and Johannes J. Fürst
Iceberg calving is a major component of the mass budget of marine- and lake-terminating glaciers. Despite increased attention to calving processes over the past few decades, large uncertainties persist in regional and global calving estimates. Although numerous empirical calving relations have been developed and implemented in glacier evolution models, iceberg calving remains a dominant source of uncertainty in future projections of marine- and lake-terminating glaciers. One of the major challenges in calving estimates is accurately tracking the ice front position at the subgrid scale. Subgrid-scale level-set methods have recently emerged as an effective approach to overcome this limitation by representing the calving front as a dynamically evolving interface.
​In this study, we present the application of a calving algorithm based on the level-set method coupled with the eigen-calving law. The method allows for a natural and robust treatment of complex topological changes at calving fronts, including retreat, advance, merging, and fragmentation. For regional application, the heterogeneity of observed retreat and glacier-specific characteristics hinders a direct spatial transfer of calving parameters. Moreover, the temporal stability of this parameter is not assured. Calibration during a single period does not guarantee good performance later. This calls for glacier-specific and transient calibration strategies to constrain calving behaviour. For this purpose, the calving algorithm is incorporated into an existing data assimilation framework that uses an Ensemble Kalman Filter. The coupled system is implemented within the Instructed Glacier Model (IGM).
We apply the model on the Kronebreen-Kongsbreen complex in Kongsfjorden, Svalbard, for the period 2000-2025. Observed calving front positions are assimilated to constrain modelled front evolution, thereby reducing uncertainty in calving front migration. By directly incorporating observational information, data assimilation avoids the need for manual, time-consuming parameter tuning. The model performs well in regions characterized by retrograde bed slopes and higher ice velocities, as in the Kronebreen complex. In contrast, the presence of bedrock ridges and narrow lateral valleys introduces additional noise into strain-based calving estimates, as observed at Kongsbreen. Despite these challenges, the results demonstrate that incorporating observational constraints via data assimilation provides an effective and scalable simulation of calving-front evolution for water-terminating glaciers.

How to cite: Prasad, V., Herrmann, O., K. c, M., R. Groos, A., and J. Fürst, J.: Till calving do us apart: Systematising data assimilation of frontal ice retreat for glacier evolution modelling of marine- and lake-terminating glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18806, https://doi.org/10.5194/egusphere-egu26-18806, 2026.

EGU26-19142 | ECS | Posters on site | CR2.4

Calibrating a Greenland ice sheet model using historical simulations between 1996-2022 

Emily Hill, G. Hilmar Gudmundsson, and Leanne Wake

Future projections of ice loss from the Greenland ice sheet are subject to large and often poorly quantified uncertainties. These arise both from uncertainties in climate forcing projections and poorly constrained processes in ice sheet models. Ice-sheet model initialisation, in particular, is a major contributor to projection uncertainty. Here, we aim to calibrate a Greenland-wide ice sheet model configuration that replicates the recent trend (1996--2022) in observed changes in ice speed and thickness. Firstwe generate an ensemble of simulations using the ice-sheet model Úa, each forced with datasets of surface mass balance and ice front positions, and input parameter values sampled from prior probability distributions. This ensemble is then used to train a surrogate model, designed to emulate the temporal- and spatially integrated combined misfit between observed and modelled changes in ice speed and thicknessWe then use this emulator for Bayesian inference to determine the posterior model parameter distributions needed to minimise the misfit between observed and modelled quantities of interest and ultimately best replicate the observed trend in Greenland ice sheet mass loss. By calibrating the model in such a way, we can reduce the uncertainties in forward-projections and have confidence in the predictive capabilities of our model. 

How to cite: Hill, E., Gudmundsson, G. H., and Wake, L.: Calibrating a Greenland ice sheet model using historical simulations between 1996-2022, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19142, https://doi.org/10.5194/egusphere-egu26-19142, 2026.

EGU26-19218 | ECS | Orals | CR2.4

A numerical stabilisation scheme for the Shallow Shelf Approximation 

A. Clara Henry, Tilda Westling Dolling, and Josefin Ahlkrona

Ice-flow modelling continues to be challenging due to the need to balance computational efficiency with physical complexity, a choice that directly affects the accuracy of sea-level projections. Several studies have successfully introduced numerical stabilisation schemes to Stokes models that reduce the stiffness of the system of equations by predicting the ice geometry at the next time step, allowing for larger time-step sizes without loss of accuracy (Durand et al., 2009, Löfgren et al., 2022, Henry et al., 2025). However, the high physical complexity of Stokes models nonetheless renders them infeasible in large-scale simulations, in part due to memory restrictions.

To address this, we introduce the Thickness Stabilisation Scheme (TSS) for the Shallow Shelf Approximation (SSA). This numerical stabilisation scheme is constructed by modifying the momentum equations with terms that predict the ice thickness at the next time step, thereby also reducing the stiffness of the problem. In order to investigate the accuracy and efficiency of TSS, we perform numerical experiments of idealised ice shelves. The results show that the inclusion of the TSS allows for a significantly larger time-step size. The improved efficiency of SSA simulations through the inclusion of the TSS enables the reallocation of computational resources towards increased spatial resolution and greater physical complexity.

Durand, O. Gagliardini, B. de Fleurian, T. Zwinger, and E. Le Meur. Marine ice sheet dynamics: Hysteresis and neutral equilibrium. Journal of Geophysical Research, 114(F3):F03009, 2009.

Löfgren, J. Ahlkrona, and C. Helanow. Increasing stable time-step sizes of the free-surface problem arising in ice-sheet simulations. Journal of Computational Physics: X, 16:100114, 2022.

A.C.J. Henry, T. Zwinger, and J. Ahlkrona. Grounding-line dynamics in a Stokes ice-flow model: Improved numerical stability allows larger time steps. EGUsphere, 2025.

How to cite: Henry, A. C., Westling Dolling, T., and Ahlkrona, J.: A numerical stabilisation scheme for the Shallow Shelf Approximation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19218, https://doi.org/10.5194/egusphere-egu26-19218, 2026.

EGU26-19880 | ECS | Posters on site | CR2.4

Projected Glacier Mass Change in High Mountain Asia Through 2100 Using the Ice-sheet and Sea-level System Model 

Javed Hassan, Gong Cheng, Helene Seroussi, Mathieu Morlighem, and Shfaqat Abbas Khan

High Mountain Asia (HMA) glaciers are critical for downstream water resources and are an increasing contributor to global sea level rise. Yet, their 21st century evolution remains uncertain because of complex topography, heterogeneous climate forcing, and limited observational constraints. Ongoing glacier mass loss reflects a shift in their buffering capacity, with consequences for the timing and reliability of downstream meltwater supply, as well as for the stability of glacierized landscapes. Quantifying this glacier response requires physically based projections of glacier evolution that adequately capture ice flow and surface processes. Existing regional projections rely on simplified flow-line, shallow-ice flow models approximating ice-dynamic processes. In this study, we simulate the glacier mass change across HMA until the end of 2100 using the Ice-sheet and Sea-level System Model (ISSM). We use a MOno-Layer Higher-Order (MOLHO) ice flow approximation on a non-uniform triangular finite-element mesh at high spatial resolution (30–500 m), locally refined based on present-day observed ice velocities. Basal friction coefficients are inferred through inverse modeling by minimizing the misfit between observed and modeled surface velocities, with independent calibration performed for each HMA subregion using observations from 2022. We use a temperature index method for surface mass balance (SMB) that explicitly accounts for the spatial distribution of supraglacial debris cover. SMB is calibrated using geodetic estimates based on stereo-imagery for the period of 2000 to 2020. We project the glaciers evolution under SSP1-2.6, SSP2-4.5, SSP3-7.0, and SSP5-8.5 climate scenarios, using bias corrected climate forcing from five CMIP6 global climate models referenced to ERA5-Land. Our results show that all regions experience mass loss by 2100, but hightlight pronounced spatial heterogeneity in glacier mass change across High Mountain Asia, with strongly varying magnitudes across subregions and climate scenarios. Under the low-emission scenario, projected mass loss remains between 11–40% compared to the glacier mass during 2000, whereas high-emission scenarios lead to substantial ice loss across most regions, ranging between 42–74% in regions such as Nyainqentanglha, Pamir, and eastern Hindu Kush. These results provide improved projections of HMA glacier change and offer valuable insights for assessing future water availability and supporting sustainable water-resource management in High Mountain Asia.

How to cite: Hassan, J., Cheng, G., Seroussi, H., Morlighem, M., and Khan, S. A.: Projected Glacier Mass Change in High Mountain Asia Through 2100 Using the Ice-sheet and Sea-level System Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19880, https://doi.org/10.5194/egusphere-egu26-19880, 2026.

EGU26-20081 | ECS | Orals | CR2.4

Modeling subglacial drainage including ice uplift and free-surface flow in 2D 

Sandra Wells, Ivan Utkin, and Mauro Werder

Numerical models of subglacial drainage have evolved to combine both distributed and channelized drainage in two dimensions, and have enabled many studies of subglacial hydrology and of its link to ice flow in glaciers and ice sheets. However, a key limitation in these models has been the inability to incorporate bounded subglacial water pressures, preventing the representation of the physical regimes of ice uplift and free-surface flow. We present a new subglacial drainage model, which extends the Glacier Drainage System (GlaDS) model to include subglacial water pressures that are bounded between atmospheric and ice overburden values. The new model includes a physics-based representation of pressurized subglacial flow, ice uplift, and free-surface flow and automatically handles the transitions between each regime domain. We demonstrate this model’s capabilities through the simulation of a rapid drainage of a supraglacial lake in Greenland, during which we observe the formation of a traveling subglacial water blister inducing ice uplift, and the partial emptying of the subglacial space at the glacier terminus near the end of the drainage.

How to cite: Wells, S., Utkin, I., and Werder, M.: Modeling subglacial drainage including ice uplift and free-surface flow in 2D, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20081, https://doi.org/10.5194/egusphere-egu26-20081, 2026.

EGU26-20196 | ECS | Posters on site | CR2.4

A new approach to model the grounding line based on mass conservation principles 

Ivan Utkin, Sandra Wells, Ciril Humbel, and Mauro Werder

The sensitivity of ice sheet dynamics to grounding line processes remains a primary source of uncertainty in sea-level rise projections. In current numerical models based on the Stokes equations, the grounding line is treated as a free boundary solved through an explicit dynamic contact formulation. This approach is highly sensitive to mesh resolution, often requiring grid spacing finer than ~200 m to ensure numerical convergence, making Stokes-based grounding line calculations computationally prohibitive for continental-scale simulations.

We present an alternative formulation for modelling the grounding line position based on the mass conservation of ice and sea water. This framework provides a physically consistent description of the ice sheet and ice shelf systems without requiring high mesh resolutions. We compare our results against existing test case suggested by Schoof (2007), show the resolutions necessary for mesh convergence and demonstrate the computational efficiency of the method.

References

1. Schoof, C. (2007). Ice sheet grounding line dynamics: Steady states, stability, and hysteresis. Journal of Geophysical Research: Earth Surface, 112(F3).

How to cite: Utkin, I., Wells, S., Humbel, C., and Werder, M.: A new approach to model the grounding line based on mass conservation principles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20196, https://doi.org/10.5194/egusphere-egu26-20196, 2026.

EGU26-20577 | ECS | Posters on site | CR2.4

Antarctic Bedrock Uncertainty 

Daantje Meijers, Emma Spezia, Johannes Sutter, Julien Bodart, and Roderik van de Wal

The future contribution of the Antarctic Ice Sheet to sea-level rise remains highly uncertain, partly due to limited knowledge of subglacial bedrock topography. Although Bedmap3 represents a major improvement over earlier compilations, substantial uncertainty persists, particularly in deep troughs beneath fast-flowing outlet glaciers.

Here, we assess how uncertainty in Antarctic bedrock topography propagates into ice-sheet projections by systematically perturbing the Bedmap3 bed within its mapped 1σ uncertainty range. Using the Parallel Ice Sheet Model (PISM), we perform transient simulations from 1950 to 3000 under constant present-day climate forcing, applying uniform and spatially correlated bed perturbations consistent with Bedmap3 uncertainty.

Bedrock uncertainty within the Bedmap3 1σ range produces an Antarctic-wide spread of approximately 0.5 m sea-level equivalent by model year 3000, highlighting bed topography as a major source of long-term projection uncertainty.

How to cite: Meijers, D., Spezia, E., Sutter, J., Bodart, J., and van de Wal, R.: Antarctic Bedrock Uncertainty, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20577, https://doi.org/10.5194/egusphere-egu26-20577, 2026.

EGU26-20608 | ECS | Orals | CR2.4

Exploration of Tunabreen surge mechanics through a fitted calving SSA model 

Bas Blank, Faezeh Nick, Johannes Oerlemans, and Adrian Luckman

Surface mass balance (SMB) estimates of glaciers in Svalbard have a relatively high degree of uncertainty despite decades of modeling and observations for the region (van Pelt et al., 2019). This is in part because the surges of marine terminating surging glaciers are complicating estimates of the mass flux towards the ocean (Schuler et al., 2020). Approximately 52% of the glaciers in Svalbard are likely or confirmed surging glaciers (Harcourt et al., 2025), making this complication to estimating the SMB common on Svalbard. The climate in Svalbard changes more rapidly than global averages (Maturilli et al., 2013; Nordli et al., 2014; Isaksen et al., 2016) but it is still unclear to what degree this affects the glaciers in Svalbard as the surge mechanics are still not well understood (Schuler et al., 2020). It does seem that the surges are increasing in frequency over the last years (Farnsworth et al., 2016). Therefore, it is hard to give projections into the future on how glaciers in Svalbard will evolve over the next 50 to a 100 years.

In our study we have looked at Tunabreen, a marine terminating surging glacier that has surge twice in the last 25 years. We use Sentinal-1-based velocity data and digital elevation models (ArticDEMs) to analyze the last surge of Tunabreen. These data show that the surge starts at the terminus and moves up in several distinct phases.

This knowledge is used to fit a calving flowline SSA model to replicate Tunabreen behavior over the last 25 years. The SSA model is based on the model from (Nick et al., 2010) with an adaptable mesh to accommodate a moving terminus as a consequence of calving. Furthermore, the model is adapted from its original form to incorporate the boundary conditions for a grounded marine terminating glacier. The calving law is based on the observed relation between water temperature and terminus retreat (Luckman et al., 2015). To force the model, we used model data of the last 25 years from ERA5-LAND for the air temperature and water temperature.

As such our model is able to replicate the evolution of Tunabreen over the last 25 years to provide insight in the possible surging mechanisms. It shows that a combination from calving, that initiated the surging, as well as subsurface hydrology sustaining the surge, leads to the typical behavior observed at Tunabreen. Using the fitted model, we can estimate how Tunabreen will evolve in the next few decades and what the effect of different climate forecast models or possible pinning points in the bedrock may have on it.

How to cite: Blank, B., Nick, F., Oerlemans, J., and Luckman, A.: Exploration of Tunabreen surge mechanics through a fitted calving SSA model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20608, https://doi.org/10.5194/egusphere-egu26-20608, 2026.

EGU26-21985 | ECS | Orals | CR2.4

Is Coupled Ice–Ocean Modeling Needed to Improve Projections of Thwaites Glacier? 

Benjamin Getraer, Mathieu Morlighem, and Daniel Goldberg

Thwaites Glacier, the West Antarctic marine giant at the center of the fastest-retreating sector of the ice sheet, has been a top priority for projections of future sea level rise since observations of its ongoing mass loss were first recognized in the mid-2000’s. The observed retreat at Thwaites Glacier is thought to be strongly influenced by the intrusion of warm circumpolar deep water (CDW) onto the continental shelf, where CDW temperature, thermocline depth, and circulation control the delivery of heat to the ice shelf and drive basal melting. This hypothesized control on retreat has led to a push to improve the source of melt rate data used in forward simulations of Thwaites, ranging from advances in observations of melt to the development of fully coupled ice–ocean models which allow for realistically responsive ocean circulation. After over a decade into the effort to couple ice sheet models and general circulation models, we ask: Is Coupled Ice–Ocean Modeling Needed to Improve Projections of Thwaites Glacier? 

We present new experimental results from a coupling of the Ice-sheet and Sea-level System Model (ISSM) and the Massachusetts Institute of Technology general circulation model (MITgcm), examining the evolution of Thwaites over the 21st century. We test the response of ice loss and grounding line retreat to future climate scenarios, thermocline depth, and periodic variability in thermocline depth on inter-annual to decadal timescales, in one of the largest sensitivity testing experiments to date. Our results show that for periods of at least decadal signals, capturing realistic variability in melt rates does not have a significant impact on the current trajectory of Thwaites’ ice loss. While error in melt rates over longer timescales, due to error or uncaptured trends in thermocline depth and resulting heat flux, can impart substantive bias into the projections of mass loss, in our model these accumulate to a relative bias of less than 10% by 2100—an absolute bias on the order of 1 to 2 mm. Significantly, the overall trends of mass loss and patterns of grounding line retreat over this time period are broadly similar in our model to uncoupled schemes. Integrating these results with past work, we argue that coupled modeling, while a powerful tool with utility in other problems, should not be prioritized as an area of research necessary to improve current projections of mass loss from Thwaites Glacier.

How to cite: Getraer, B., Morlighem, M., and Goldberg, D.: Is Coupled Ice–Ocean Modeling Needed to Improve Projections of Thwaites Glacier?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21985, https://doi.org/10.5194/egusphere-egu26-21985, 2026.

EGU26-22583 | Orals | CR2.4

A second-order implicit time-stepping scheme for full-Stokes ice-sheet models 

Josefin Ahlkrona, Clara Henry, and André Löfgren
We present a second-order implicit method for coupling the free surface and velocity in full-Stokes ice-sheet models [1]. The method enables the use of very large time steps, in contrast to standard implicit solvers, which diverge in this regime.
Convergence of the implicit solver is achieved by adding and subtracting two so-called FSSA (Free Surface Stabilization Approach) stabilization terms. Unlike previous FSSA formulations, the stabilization terms do not affect the accuracy of the final solution, as they vanish upon convergence. This stabilized implicit iteration scheme is then used to construct a second-order backward differentiation formula (BDF2) time-integration method.
The method is implemented and evaluated on idealized and realistic ice-sheet test cases in Elmer/Ice and Biceps, demonstrating improved stability, accuracy, and computational efficiency. While developed for glaciological applications, the approach is easy to implement and directly applicable to other viscous free-surface Stokes problems.
 
[1] Ahlkrona, J., Henry, A. C. J., and Löfgren, A.: A fully implicit second-order method for viscous free-surface Stokes flow – application to glacier simulations, EGUsphere, 2025, 1–24, https://doi.org/10.5194/egusphere-2025-4359

How to cite: Ahlkrona, J., Henry, C., and Löfgren, A.: A second-order implicit time-stepping scheme for full-Stokes ice-sheet models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22583, https://doi.org/10.5194/egusphere-egu26-22583, 2026.

EGU26-2856 | Orals | CR2.5

Modelling and Parameterisation of Ice-Shelf Melting in the Amundsen Sea 

Paul Holland, Adrian Jenkins, David Bett, Suzanne Bevan, and Adrian Luckman

The rapid ice loss from the Amundsen Sea sector of West Antarctica is a major contributor to global sea-level rise, and is driven by changes in ocean melting. In this study we use high-resolution ocean simulations to understand the mechanisms controlling ice-shelf melting in the eastern Amundsen Sea. Melting is focussed on four ‘hot spots’ of melting of the deep ice where the main glacier trunks cross the grounding line. Secondary areas of elevated melting occur beneath the associated buoyant meltwater plumes, which are guided by ice topography and Coriolis force. The simulations are then used to test simple local parameterisations of melting. The best parameterisation expresses melt rate as a simple function of ocean temperature to the power 3/2, ice slope to the power 1/2, and tapered to zero near the grounding line. This matches the simulated melting with a spatial correlation of r2=0.65, capturing deep melting near the grounding line but omitting melting by the buoyant plumes. This parameterisation also broadly captures the strong melting feedbacks that appear when the model is applied to possible future ice geometries. This leads us to speculate that simple local melting parameterisations may be sufficient in ice sheet forecasts wherever ice shelf buttressing is focussed near the grounding line (such as Thwaites Glacier), but may be inadequate in regions where melting beneath shear margins controls buttressing (such as Pine Island Glacier).

How to cite: Holland, P., Jenkins, A., Bett, D., Bevan, S., and Luckman, A.: Modelling and Parameterisation of Ice-Shelf Melting in the Amundsen Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2856, https://doi.org/10.5194/egusphere-egu26-2856, 2026.

EGU26-3174 | Posters on site | CR2.5

Wind-driven coastal polynya variability drives decadal ice-shelf melt variability in the Amundsen Sea 

Michael Haigh, Paul Holland, Thomas Caton Harrison, and Pierre Dutrieux

The ice shelves in the Amundsen Sea, West Antarctica, are being melted rapidly by warm Circumpolar Deep Water (CDW), causing sea-level rise. Variability in ice-shelf melting is controlled by the speed of a shelf-break undercurrent which transports CDW from the deep ocean onto the continental shelf. We study decadal variability of the undercurrent and ice-shelf melting using new regional ice-ocean model perturbation experiments. The perturbation experiments suggest that the undercurrent decadal variability is controlled by variable coastal sea-ice freshwater fluxes, these driven by winds mechanically opening and closing coastal polynyas. With the perturbation experiments we also quantify a positive feedback mechanism between the undercurrent and ice-shelf melting which is responsible for 25% of their decadal variability.

How to cite: Haigh, M., Holland, P., Caton Harrison, T., and Dutrieux, P.: Wind-driven coastal polynya variability drives decadal ice-shelf melt variability in the Amundsen Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3174, https://doi.org/10.5194/egusphere-egu26-3174, 2026.

EGU26-3797 | ECS | Orals | CR2.5

Calibration of a coupled ice-ocean model using observations of ice dynamics and basal melt in West Antarctica 

Brad Reed, Jan De Rydt, Kaitlin Naughten, and Daniel Goldberg
Coupled ice sheet-ocean models are increasingly used to investigate the complex interactions between ice dynamics and ocean forcing in West Antarctica, yet uncertainties in model parameters limit confidence in long-term sea-level projections. Among these parameters, ocean-model melt rates are typically calibrated using only basal melt observations for static ice-shelf geometries, neglecting feedbacks associated with evolving ice geometry, particularly in the Amundsen Sea sector.
   
Here, we calibrate a fully coupled ice sheet-ocean model using an ensemble of simulations constrained by spatial observations of basal melt rates and changes in ice speed and thickness over a historical period. This represents the first calibration to jointly incorporate oceanic and glaciological observations for tuning melt-rate parameters. To match the historical observations of ice dynamical changes, the transient-coupled calibration requires enhanced melt near the grounding line, highlighting the sensitivity of ice dynamics to localized ocean forcing.
   
Using the historically-calibrated model, we provide century-scale projections of sea-level contribution under two climate scenarios. In a warm RCP8.5 scenario, the transient-coupled calibration increases projected 2100 sea-level rise by 10 mm relative to a melt-only calibration, exceeding the 7 mm difference due to a change in climate forcing alone. These findings underscore the critical importance of jointly constraining oceanic and glaciological observations in model calibration. Further improvements will include extending the hindcast period, testing additional forcing scenarios, and calibrating ice-sheet model parameters.

How to cite: Reed, B., De Rydt, J., Naughten, K., and Goldberg, D.: Calibration of a coupled ice-ocean model using observations of ice dynamics and basal melt in West Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3797, https://doi.org/10.5194/egusphere-egu26-3797, 2026.

EGU26-6678 | ECS | Posters on site | CR2.5

Warm mode melt impact on ice dynamics in Antarctica 

Rosie Archer, Ronja Reese, Lena Nicola, and Ricarda Winkelmann

The Antarctic Ice Sheet is losing mass, a large part of which is due to ocean melting under ice shelves. Current projections from the ISMIP6 project show a gradually warming ocean forcing in currently cold cavities, but there is a growing literature that this may not be an accurate representation of how the temperatures beneath the ice shelves will change. Instead, the cold Antarctic ice shelves – like Filchner-Ronne or Ross – are expected to experience an intrusion of warmer circumpolar deep water under strong climate forcings. This has the potential to shift the regime of the Antarctic basins from cold to warm states, leading to increased melt rates. 

Here, we focus on three of the currently cold-based basins, namely Filchner-Ronne, Amery, and Ross. Using the literature of likely timings for regime shifts for each of these cavities, we investigate how an immediate temperature change at these timings compares to the gradual warming beneath the cavities modelled in the ISMIP6 simulations. We create an ocean forcing using the warm mode temperature anomalies from Nicola et al., (2025) to represent the regime change in these basins and run simulations using the numerical ice sheet models Ua and PISM, coupled with the ice sheet cavity box model PICO. Then, we compare the model outputs to simulations using the original CMIP6 ocean forcing.

Nicola, L., Reese, R., Kreuzer, M., Albrecht, T., and Winkelmann, R.: Bathymetry-constrained warm-mode melt estimates derived from analysing oceanic gateways in Antarctica, The Cryosphere, 19, 2263–2287, https://doi.org/10.5194/tc-19-2263-2025, 2025.

How to cite: Archer, R., Reese, R., Nicola, L., and Winkelmann, R.: Warm mode melt impact on ice dynamics in Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6678, https://doi.org/10.5194/egusphere-egu26-6678, 2026.

EGU26-6776 | ECS | Orals | CR2.5

Resolving glacier–fjord interactions using observations of 3-dimensional fjord circulation, plume activity, and glacier dynamics 

Andrea Kneib-Walter, Donald Slater, Armin Dachauer, and Andreas Vieli

Interactions between tidewater glaciers and fjord waters play a key role in Greenland Ice Sheet mass loss. However, many of the underlying processes remain hidden beneath the fjord surface. In particular, the coupling between subglacial meltwater discharge, plume formation, fjord circulation, ice mélange conditions, and glacier dynamics is poorly constrained due to the difficulty of obtaining temporally and spatially highly resolved observations in these environments. This lack of observations limits our ability to resolve glacier-fjord interactions, resulting in considerable uncertainties in mass loss projections.

We address this challenge using an extensive time series of terrestrial radar interferometry (TRI) observations collected at the tidewater glacier Eqalorutsit Kangilliit Sermiat in South Greenland. Using this dataset, we analyse meltwater plume activity, ice mélange conditions in the fjord, glacier motion, calving activity, and 3-dimensional fjord circulation at minute-scale temporal resolution over several weeks, presenting an integrated observational view of the glacier–fjord system, including processes occurring below the waterline.

Fjord circulation is inferred using an autonomous iceberg-tracking framework that derives 3-dimensional flow patterns from the motion of icebergs spanning a wide range of sizes. Combining trajectory data with iceberg drafts, estimated from TRI-derived elevation models, allows circulation to be resolved across different water-depth layers within the ~300 m deep fjord. These observations are evaluated alongside fjord stratification measured by CTD profiles. The results reveal a highly complex circulation that varies strongly with water depth, time, and location in the fjord. Icebergs can even move in opposite directions depending on their draft and the dominant current acting on them. These observations are consistent with modelled fjord circulation, placing the measurements within a process-based framework.

Subglacial meltwater discharge and plume dynamics are investigated using a newly developed autonomous plume-detection algorithm applied to terrestrial radar data. Temporal changes in plume surface area are combined with melt modelling and subglacial hydrological routing to estimate meltwater fluxes entering the fjord. In parallel, ice mélange conditions are quantified using time-lapse imagery and radar backscatter, providing insight into mélange rigidity, its temporal evolution, and its influence on calving and terminus dynamics. On short (subdaily) timescales, plume area does not directly reflect discharge magnitude, as ice mélange conditions strongly control whether meltwater reaches the surface. Over longer (daily) timescales, however, plume size evolution generally agrees with estimated discharge variability.

Overall, these results advance our understanding of how subglacial discharge–driven circulation influences ocean-driven melting and glacier terminus stability, with important implications for projecting Greenland Ice Sheet mass loss and assessing fjord ecosystem responses under ongoing climate change.

How to cite: Kneib-Walter, A., Slater, D., Dachauer, A., and Vieli, A.: Resolving glacier–fjord interactions using observations of 3-dimensional fjord circulation, plume activity, and glacier dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6776, https://doi.org/10.5194/egusphere-egu26-6776, 2026.

EGU26-6816 | ECS | Posters on site | CR2.5

Insights into ocean mixing processes driving ice shelf melting from highly resolved simulations  

Sam Hartharn-Evans, Jan De Rydt, Charlie Lloyd, Magda Carr, and Adrian Jenkins

The melting of ice shelves into the ocean plays a major role, and is a key source of uncertainty, on sea level rise projections. Under ice shelves, meltwater moves upslope, setting up a stratified shear flow with the warmer, but critically saltier, ocean beneath, regulating the transfer of heat between ice and the ambient ocean. These stratified flows are incredibly difficult to access in situ, and so research has focussed on the use of numerical modelling, laboratory experiments and analytical models to understand these processes, each with their own assumptions, advantages and limitations.

Here we present novel direct numerical simulations that represent this basal melt process with highly resolved (sub-millimeter resolution) simulations that reveal this shear flow evolves as a unique mixed mode shear instability. Unusually, the combined input of buoyancy, and a solid boundary leads to paired Kelvin Helmholtz and Holmboe instabilities, which prove highly effective at mixing the water column. Due to the restoring effect of the boundary forcing, a cycle of growth, instability, turbulent mixing, and re-stabilisation is observed. Results for a non-rotating framework with equal diffusivities for heat and salt are contrasted to simulations with added complexity, including rotation and double-diffusive processes. These findings suggest that current ice-ocean parametrisations are fundamentally built on assumptions for stratified flow instabilities that may differ from these simulations, with potential implications for the turbulent transfer of heat and salt and ultimately basal melt rates. 

How to cite: Hartharn-Evans, S., De Rydt, J., Lloyd, C., Carr, M., and Jenkins, A.: Insights into ocean mixing processes driving ice shelf melting from highly resolved simulations , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6816, https://doi.org/10.5194/egusphere-egu26-6816, 2026.

Conventional basal melt parameterisations for ice shelf basal melting typically calculate melt rates as a direct function of ambient ocean properties, effectively bypassing the internal physics of the ice-ocean boundary layer (IOBL). This simplification often leads to significant overestimations of melting, particularly when stable stratification is present.

The core of our framework is a set of parametric equations that computes melt rates after determining the thermal driving within the boundary layer by resolving:

  • Heat transfer from the ambient ocean into the boundary layer.
  • Heat transfer from the boundary layer to the ice-ocean interface.

By resolving the internal physics of the boundary layer, this framework provides a valuable tool for process studies, allowing for a deeper investigation into how different forcing mechanisms influence basal melting. We will discuss the physics behind this framework and how this framework can be developed in the future by including more physics to improve the representation of ice-ocean interactions in large-scale climate models.

How to cite: T. Pillai, J. and Jenkins, A.: Capturing Ice-Ocean Boundary Layer Physics over Dynamically Stable Pycnoclines: The Mechanics of a Parameterisation Framework for Basal Melting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7574, https://doi.org/10.5194/egusphere-egu26-7574, 2026.

EGU26-9851 | ECS | Orals | CR2.5

Synchronous velocity change in response to ocean forcing on marine-terminating glaciers in central- and south-eastern Greenland (2014–2025) 

Mae Evans, Anna Hogg, Trystan Surawy-Stepney, Benjamin Wallis, Ross Slater, and Richard Rigby

Marine-terminating glaciers in central and southeast Greenland are major contributors to Greenland’s dynamic mass loss and include several of its fastest-flowing outlet glaciers. Ice-ocean interactions have a strong control on the dynamics of marine-terminating glaciers, yet observations of region-wide glacier responses to ocean forcing remains limited. Recent dynamic changes across this sector have largely been studied at smaller spatial scales, limiting our understanding of coherent and more widespread regional scale behaviour and responses to environmental forcing.

Here, we use more than a decade of Sentinel-1 satellite observations to measure ice velocity change on 66 marine-terminating glaciers, between 2014 and 2025 and access the impact of ocean and sea-ice anomalies on glacier dynamics. We observe a widespread and pronounced speedup on ice streams in this region with synchronous acceleration beginning in 2016 and peaking around 2020. Speedup is observed on 43 of the 66 glaciers with the majority of speedup exceeding that observed in the mid 2000’s. Six glaciers more than double in speed and several ice streams reach their fastest speeds in at least two decades. This period of acceleration is followed by a widespread deceleration after 2020, although most glaciers remain faster than their pre-2016 velocities.

We investigate the impact of ocean and atmospheric forcing on the ice velocity change to better understand the drivers. Our results indicate that the timing of this region wide acceleration coincides with anomalously warm surface and subsurface ocean temperatures and a prolonged reduction in regional sea-ice concentration, suggesting that ocean driven forcing may have synchronised glacier responses.

These results show that recent ocean driven dynamic change in central and southeast Greenland has been larger and more spatially extensive than previously recognised, highlighting the susceptibility of these glaciers to rapid, synchronous change and the importance of ice-ocean interactions. The sensitivity of the region to ocean forcing shows that this marine terminating part of the Greenland ice sheet is delicately coupled with its environment and should be closely monitored in the future.

How to cite: Evans, M., Hogg, A., Surawy-Stepney, T., Wallis, B., Slater, R., and Rigby, R.: Synchronous velocity change in response to ocean forcing on marine-terminating glaciers in central- and south-eastern Greenland (2014–2025), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9851, https://doi.org/10.5194/egusphere-egu26-9851, 2026.

EGU26-10158 | ECS | Posters on site | CR2.5

A novel finite element model for simulating fjord circulation 

Jonathan Wiskandt, Lukas Lundgren, Josefin Ahlkrona, and Johan Nilsson

Basal melt of marine terminating glaciers is a key uncertainty in predicting the future climate and the evolution of the Greenland Ice Sheet. Detailed observations about the distribution of melt at Greenland’s glaciers and the ocean circulation in the adjoining fjords and specifically at the ice-ocean interface, are rare, due to the remoteness of the regions of interest. Hence, we rely heavily on models to get deeper insights into the processes in the fjords, underneath the ice shelves and at the ice-ocean interface. 

We present a novel Finite Element Model used to simulate the circulation in North Greenland's Sherard Osborn Fjord. Thanks to the finite elements the model can accurately represent fjord bathymetry and ice base geometry at the meter scale. A novel, symmetric, tensor-based viscosity formulation, using a residual-based method (residual viscosity), allows for high resolutions (meters) with minimal artificial viscosity and sharp gradients, while keeping computational times low. 

A high resolution representation of the sill in Sherard Osborn Fjord enables a more accurate simulation of the inflow of warm Atlantic Water towards the glacier. The more realistic representation of the ice base geometry and the high resolution allows us to model the distribution of melt rate underneath the ice shelf of Ryder Glacier in great detail, which can lead to better estimates of total melt rate. Furthermore, the high resolution and novel implementation of residual viscosity in the model enables an accurate simulation of the melt water plume with sharper gradients between the plume and the ambient water due to the absence of excess artificial viscosity and diffusivity.

In addition to the high resolution 2D simulations we are currently working on a 3D simulation using realistic ice base geometry and fjord bathymetry from Ryder Glacier and Sherard Osborn Fjord.

How to cite: Wiskandt, J., Lundgren, L., Ahlkrona, J., and Nilsson, J.: A novel finite element model for simulating fjord circulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10158, https://doi.org/10.5194/egusphere-egu26-10158, 2026.

EGU26-11623 | ECS | Posters on site | CR2.5

Towards ocean model simulations of the Southern Ocean and Antarctic ice shelf cavities forced by CMIP historical climate data 

Alethea S. Mountford, Ronja Reese, Adrian Jenkins, Christopher Y.S. Bull, Robin Smith, Birgit Rogalla, and Kaitlin A. Naughten

Ocean-driven melting of ice shelves is the primary cause of ice loss in Antarctica, ultimately leading to global sea-level rise. However, there is still much uncertainty over the interactions between physical processes that lead to this ocean-driven melting, such as the role of climate-driven wind changes, increasing air temperatures and changes in freshwater fluxes, such as precipitation and ice sheet runoff. The timescales over which the ice loss will occur and the subsequent potential for sea-level rise are also areas of uncertainty in need of further investigation. At present, many ocean models that provide data to drive ice sheet models, such as those in CMIP, do not accurately represent ocean conditions around Antarctica, for example due to low model resolution or a very simplified representation of ice shelves. Ice sheet models then use empirical schemes based on remote offshore ocean temperatures to estimate the ice shelf melt from CMIP models. As such, predictions of potential sea-level rise that depend on these simulations may in turn not be accurate. Improving the representation of ocean water masses and circulation on the continental shelves and underneath the ice shelves around Antarctica would therefore be a key improvement for forcing ice sheet models that are used for predicting ice loss related sea-level rise.

We present the results from a 1/4º resolution circum-Antarctic ocean model with a representation of ice shelf cavities and ice shelf melt, run over the historical period of 1850-2020, forced with UKESM 1.2 CMIP6 outputs. These historical outputs, alongside simulations to be run with projected SSP5-8.5 forcing, will aim to provide a better representation of water masses around Antarctica to force ice sheet models. Using these, we plan to further our understanding of the physical processes that drive ocean-driven melt, and derive climate transfer functions that can bridge the gap between ice sheet models and coarse resolution general circulation models.

How to cite: Mountford, A. S., Reese, R., Jenkins, A., Bull, C. Y. S., Smith, R., Rogalla, B., and Naughten, K. A.: Towards ocean model simulations of the Southern Ocean and Antarctic ice shelf cavities forced by CMIP historical climate data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11623, https://doi.org/10.5194/egusphere-egu26-11623, 2026.

EGU26-12063 | Orals | CR2.5

Wave-induced erosion at ice-shelf fronts under irregular and breaking-wave conditions 

Wenjun Lu, Dominique Mouaze, Behnam Ghadimi, Marianne Font, Rémi Lambert, Shovon Jubair, Lotte Wendt, Harvey Goodwin, Geir Moholdt, Raed Lubbad, and Sveinung Løset

Wave–ice interactions are widely recognised as one of several mechanisms contributing to ice-shelf front retreat. However, their role at small spatial and temporal scales remains difficult to quantify, particularly under breaking-wave conditions. Here, we investigate wave-induced erosion at the ice–ocean interface by combining satellite observations, laboratory experiments, and simplified, scale-aware modelling.

Ice-front retreat during the austral summer of 2024 is analysed using Sentinel-1 SAR imagery. Multiple coastline-tracking methods are applied to quantify the spatial and temporal variability of the ice front. The observations reveal periodic collapse events that tend to be temporally synchronised with elevated wave activity. This points to a strong link between wave forcing and short-term ice-front instability.

To interpret these observations, we extend classical wave-induced melting formulations by introducing a first-order, breaking-aware modelling procedure. Wave shoaling and depth-limited breaking are accounted for by tracking the evolution of wave height with water depth and by using the near-breaking horizontal particle velocity as the effective velocity scale driving heat transfer at the ice–water interface. This simple approach captures the enhancement of wave-induced erosion associated with irregular and incipiently breaking waves, while remaining computationally efficient.

The formulation is first evaluated using small-scale laboratory experiments conducted at the University of Caen, where harmonic, non-breaking waves interact with an ice cube. In this controlled experiment, measured erosion rates agree well with theoretical predictions, confirming the validity of classical approaches when wave breaking is absent. When applied to field conditions at Fimbulisen, however, the breaking-aware formulation substantially increases predicted erosion rates relative to classical theory but still systematically underestimates observed retreat. The remaining discrepancy points to unresolved turbulence processes associated with fully developed breaking and motivates the need for more advanced theoretical and experimental treatment of wave-breaking-induced mixing at the ice–ocean interface.

How to cite: Lu, W., Mouaze, D., Ghadimi, B., Font, M., Lambert, R., Jubair, S., Wendt, L., Goodwin, H., Moholdt, G., Lubbad, R., and Løset, S.: Wave-induced erosion at ice-shelf fronts under irregular and breaking-wave conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12063, https://doi.org/10.5194/egusphere-egu26-12063, 2026.

EGU26-14670 | ECS | Orals | CR2.5

Impact of ice mélange thickness on mélange melt rate in Greenland’s glacial fjords 

Lokesh Jain, Donald Slater, and Peter Nienow

In recent decades, Greenland’s marine-terminating glaciers have retreated and accelerated, contributing significantly to global sea level rise. The presence of an ice mélange, and its associated buttressing force on a glacier terminus, has a significant impact on glacier advance and retreat. The buttressing force is modulated by the thickness of the ice mélange, which in turn is influenced by mélange melt rate, but our understanding of ice mélange melting remains limited. In particular, a quantitative understanding of how the thickness of an ice mélange impacts melt rates is lacking.

Here, we model the melting of ice mélange by the ocean using the ocean model MITgcm to simulate the water flow in the first 15km down-fjord from the calving front, focusing specifically on the relationship between the melt rate and the mélange thickness. Ice mélange is represented in the model by cuboid icebergs that are thermodynamically active, divert the fluid flow and represent a range of sizes to reflect realistic observed iceberg distributions. We find that melt rate generally increases with mélange thickness and is particularly sensitive to mélange thickness at thicknesses below approximately 100 metres. Based on these simulations, we develop a parameterisation for mélange melt rate as a function of subglacial discharge, oceanic thermal forcing and mélange thickness. We then apply this parameterisation around Greenland to the ice mélange at 27 glaciers. We estimate melt rates in the range 0.05 – 0.92 m/d, which is comparable with observational estimates, and extract the dominant factors that control glacier-to-glacier variability in mélange melt. The development of this parameterisation is a key step in advancing our understanding of the dynamics of ice mélange and enabling a representation of ice mélange in larger climate and ice sheet models.

How to cite: Jain, L., Slater, D., and Nienow, P.: Impact of ice mélange thickness on mélange melt rate in Greenland’s glacial fjords, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14670, https://doi.org/10.5194/egusphere-egu26-14670, 2026.

EGU26-16663 | Orals | CR2.5

The impact of submesoscale ocean eddies on the basal melting of ice shelves using high-resolution simulations 

Catherine Vreugdenhil, Wangpeng Gui, Bishakhdatta Gayen, and Ankit Bhadouriya

The ocean-driven melting of ice shelves is a key impact on ice shelf mass loss and on the stability of the Antarctic ice sheet. However, knowledge is incomplete on the impact of ocean processes on the basal melting of ice shelves, in particular the effects of submesoscale processes. Inspired by recent observations of an eddy beneath an ice tongue (Hancock et al., 2025), we investigate a series of simulations to better understand the effect of eddies on the localised melting of ice shelves. Here, we examine submesoscale eddies beneath an ice shelf using large-eddy simulations that resolve all but the smallest scales of turbulence. In order to resolve the thin mm-scale layers immediately below the ice, the domain size is limited and the eddies are scaled down to be metres in size. The dynamical regime in which these simulations operate is relevant for the ocean application, hence we can relate our simulations to observations and results from large-scale ocean models. We initialise our simulations with a salinity front beneath an ice shelf, with different chosen temperature profiles to match cold and warm ice shelf cavities. Once the simulations are initiated, the front breaks into submesoscale eddies. Our results show that anticyclonic eddies enhance the ice melting by upwelling warm underlying waters. In contrast, cyclonic eddies moderate the melting by downwelling cool meltwater. Our simulated results compare favourably with the existing observations and the application to other ocean regions is also discussed. 

How to cite: Vreugdenhil, C., Gui, W., Gayen, B., and Bhadouriya, A.: The impact of submesoscale ocean eddies on the basal melting of ice shelves using high-resolution simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16663, https://doi.org/10.5194/egusphere-egu26-16663, 2026.

EGU26-19455 | Posters on site | CR2.5

HAs the Greenland Ice Sheet Reached Peak Ice Discharge - HAGRID 

Peter Nienow and Hannah Picton

During recent decades, the glaciological community has become familiar with statements in numerous papers, and high-profile reports, highlighting that ‘Greenland’s marine-terminating glaciers are retreating, accelerating and thinning’. However, while the vast majority of Greenland’s 200+ marine terminating glaciers have both retreated and thinned in recent decades, and many have certainly accelerated, the net impact of these changes on ice mass flux has been somewhat limited and extremely variable between individual glaciers. Indeed, a brief consideration of dynamic ice-flux data suggests that with the exception of a ~10% increase between 2000 and 2005, ice flux from these systems has shown minimal increase (<2%) in the two decades since the early millennial dynamic shift with the contribution from the largest 15 outlet glaciers remaining largely invariant. This observation not only brings in to question the suggestion of ubiquitous acceleration; it also raises the question that if one considers ice-flux, which is the most critical determinant for future sea-level rise, have we already or will we shortly reach peak ice flux from the Greenland Ice Sheet? It is clear that at some point, and in a corollary with ‘peak water’ in deglaciating valley glaciers, that each tidewater glacier will reach peak discharge and that this will occur prior to each glacier retreating on to land. This paper investigates in detail recent patterns of ice-flux change, both in terms of regional variability and glacier size, in order to consider the likelihood of future acceleration in ice-mass loss via solid ice-discharge from the Greenland Ice Sheet.

How to cite: Nienow, P. and Picton, H.: HAs the Greenland Ice Sheet Reached Peak Ice Discharge - HAGRID, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19455, https://doi.org/10.5194/egusphere-egu26-19455, 2026.

EGU26-20585 | ECS | Orals | CR2.5

Spatially and Temporally Dense Grounding Lines from Bayesian Inversion of Sentinel-1 Data 

Sindhu Ramanath Tarekere, Michael Engel, Lukas Krieger, Jan Wuite, Dana Floricioiu, and Marco Körner

Grounding lines are flux gates through which ice discharges into the ocean. Their position reflects ice sheet stability, retreating landward or advancing seaward in response to changes in melting and accumulation, while also exhibiting short-term motion driven by tidal flexure of floating ice. Grounding lines derived from Differential Interferometric SAR (DInSAR) phase are generally regarded as the most accurate [1]. However, most existing datasets lack formal uncertainty estimates, even though grounding line errors directly propagate into ice discharge calculations and can substantially bias estimates of ice mass loss and sea level rise [1]. A further limitation is that DInSAR grounding lines are derived from interferograms combining three or four SAR acquisitions, such that each estimated position represents a superposition of multiple tidal states, complicating the attribution of observed displacements to specific tidal forcing.

We have developed a framework to obtain grounding line positions together with Bayesian estimates of positional uncertainty. Based on this, we generated a dense time series of grounding lines for the Larsen C Ice Shelf spanning 2019–2021, derived from Sentinel-1 line-of-sight (LOS) offsets at a temporal sampling of 6 days. The LOS offsets are part of the operational processing pipeline used by ENVEO IT to produce monthly and annual Sentinel-1 ice-velocity maps, and were computed by tracking features between consecutive SAR backscatter images [2], [3]. Grounding line positions were estimated by fitting the LOS offsets to a one-dimensional elastic beam model [4] and performing Bayesian inversion using the cross entropy based importance sampling for Bayesian updating (CEBU) algorithm [5], which allows the incorporation of external datasets as priors on model parameters. Additionally, the estimated error of the range offsets were explicitly accounted for in the inversion. The resulting dataset provides a dense time series of grounding lines which have a mean distance of 348.07 m from Sentinel-1 DInSAR grounding lines. Because the dataset is derived from SAR backscatter rather than interferometric phase, it is robust to coherence loss and can be used to fill gaps in DInSAR grounding line products over fast-flowing outlet glaciers and ice streams.

References

[1] E. Rignot, J. Mouginot, and B. Scheuchl, “Antarctic grounding line mapping from differential satellite radar interferometry: GROUNDING LINE OF ANTARCTICA,” Geophysical Research Letters, vol. 38, no. 10, 2011

[2] T. Nagler, H. Rott, M. Hetzenecker, J. Wuite, and P. Potin, “The sentinel-1 mission: New opportunities for ice sheet observations,” Remote Sensing, vol. 7, no. 7, pp. 9371–9389, 2015.

[3] J. Wuite, T. Nagler, M. Hetzenecker, and H. Rott, “Ten years of polar ice velocity mapping using Copernicus Sentinel-1,” Remote Sensing of Environment, vol. 332, p. 115 092, Jan. 2026

[4] G. Holdsworth, “Flexure of a Floating Ice Tongue,” Journal of Glaciology, vol. 8, no. 54, pp. 385–397, 1969, 1727-5652

[5] M. Engel, O. Kanjilal, I. Papaioannou, and D. Straub, “Bayesian updating and marginal likelihood estimation by cross entropy based importance sampling,” Journal of Computational Physics, vol. 473, p. 111 746, Jan. 2023

How to cite: Ramanath Tarekere, S., Engel, M., Krieger, L., Wuite, J., Floricioiu, D., and Körner, M.: Spatially and Temporally Dense Grounding Lines from Bayesian Inversion of Sentinel-1 Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20585, https://doi.org/10.5194/egusphere-egu26-20585, 2026.

EGU26-21154 | Orals | CR2.5

Quantifying melt rates in Antarctic grounding zones using flexural inversion 

Jerome Neufeld, Reefe Conley, and Paul Holland
Antarctic ice shelves in the Amundsen Sea embayment are vulnerable to rapid disintegration, the dynamics of which depend strongly on the rate of melting of the ice shelf.  In particular, melt rates in the grounding zone - where ice transiently makes contact with the bedrock - have proven difficult to measure using remote methods which rely on remote measurements of the ice freeboard and an application of the hydrostatic approximation.  Here, we extend existing remote observations of melt rates into the grounding zone by incorporating a model of the elastic flexure of ice shelves.  The numerical model is tested against existing analytical models, and then demonstrated on select ice shelves in the Amunsdsen sea embayment.  Melt rates are found which are comparable with existing hydrostatic estimates away from the grounding zone, but are more continuous within the region of transient contact with the bedrock.

How to cite: Neufeld, J., Conley, R., and Holland, P.: Quantifying melt rates in Antarctic grounding zones using flexural inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21154, https://doi.org/10.5194/egusphere-egu26-21154, 2026.

EGU26-22362 | ECS | Orals | CR2.5

Impacts of iceberg capsize-induced sudden ocean mixing on fjord circulation and glacier melt 

Oscar Tovey Garcia and Andrew Wells

The Greenland Ice Sheet loses roughly half of its mass by ice discharge at marine terminating 
glaciers. Some of the largest and fastest flowing glaciers around Greenland calve kilometre-scale 
icebergs into long, narrow and deep fjords. These enormous icebergs typically capsize, or “flip” into 
more gravitationally stable orientations, and in doing so are thought to vigorously mix the stratified 
ocean within a small region in front of the glacier front. 
We investigate the effect of sudden ocean mixing events on flow within an idealised, linearly
stratified model fjord using the Oceananigans.jl nonhydrostatic model. A large fraction of the 
available potential energy is rapidly converted to kinetic energy and radiates away as internal waves. 
These internal waves produce pulses of elevated melt rate across the entire glacier front, with 
magnitudes comparable to melt rates due to subglacial discharge plumes. On longer timescales, the 
qualitative character of the response depends on the ratio of fjord width, W, to first baroclinic 
Rossby deformation radius, R. Typical Greenland fjords have W/R between 0.5 and 2.0. Within this 
range of W/R, our model predicts the appearance of a long-lived nearly geostrophic anticyclonic 
eddy spanning the entire width of the fjord, constrained to mid-depths, in front of the glacier 
terminus. This eddy drives a sustained melt anomaly at mid-depths for many days, which may 
promote undercutting. We also investigate sensitivity to the horizontal extent of the region over 
which the fluid is mixed, and find that increasing the mixed volume beyond some critical value 
destabilises the abovementioned eddy, leading to its break up and consequently reducing the 
predicted glacier melt rate. 

How to cite: Tovey Garcia, O. and Wells, A.: Impacts of iceberg capsize-induced sudden ocean mixing on fjord circulation and glacier melt, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22362, https://doi.org/10.5194/egusphere-egu26-22362, 2026.

EGU26-1898 | ECS | PICO | CR2.6

Investigating the stability of Greenland’s outlet glaciers 

Jowan Barnes and Hilmar Gudmundsson

The Greenland Ice Sheet is the fastest growing contributor to sea level rise, due to loss of ice from its marine-terminating outlet glaciers. One of the largest of these is Helheim Glacier, located in eastern Greenland. Recent observational work suggests that Helheim could be approaching a threshold beyond which it would undergo rapid retreat. Here, we present a modelling study investigating the stability of Helheim Glacier. We seek to establish whether such a threshold exists in the future evolution of this glacier, and whether a rapid retreat event would be reversible. We approach this by initialising the model to a steady state close to the present-day geometry of the glacier, then carrying out a series of experiments to test its stability in relation to changes in atmospheric and ocean forcing. Calving front positions at the ocean interface and mass balance at the surface are perturbed incrementally, and the system allowed to reach a new steady state after each perturbation. The forcing is then reversed in order to assess whether the resulting changes to the glacier’s position and dynamics are reversible. Our methodology is demonstrated in synthetic geometries representative of Greenlandic fjord environments, in which we find a hysteresis behaviour within the system such that after a retreat of the ice front, readvance will not occur along the same pathway when the forcing is reversed. Initial results suggest that such behaviour is also present within the Helheim system.

How to cite: Barnes, J. and Gudmundsson, H.: Investigating the stability of Greenland’s outlet glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1898, https://doi.org/10.5194/egusphere-egu26-1898, 2026.

The Antarctic Ice Sheet is a major contributor to present-day sea-level rise, with most mass loss occurring through ice shelves that regulate upstream ice flow via buttressing effect. Recent widespread ice-shelf thinning, enhanced calving, and structural weakening underscore the need for long-term observations to understand ice-shelf stability and potential tipping behavior. Pine Island Glacier and its ice shelf, located in the Amundsen Sea sector of West Antarctica, have experienced sustained acceleration, thinning, and retreat since the 1970s, making this system an ideal natural laboratory for investigating ice-shelf dynamic responses to climate forcing.

Here, we investigate the dynamic evolution and stability of the Pine Island Ice Shelf (PIIS) from 2014 to 2025 using multi-source satellite remote-sensing data. While the dynamics for the PIIS for the last decade are dominated by accelerating flow, the velocity time series also reveal a deceleration of the central PIIS between 14 March 2022 and 20 January 2023. Piglet Glacier, a major tributary of the PIIS, also experienced two distinct deceleration periods between 2023 and 2025. Our analysis demonstrates that ice flow in the central PIIS and Piglet Glacier is highly sensitive to mechanical coupling along shear margins, modulated by variations in the state and configuration of dense ice mélange. In the northern sector of the ice shelf, sustained thinning, loss of pinning points, rift propagation, and a major calving event collectively indicate progressive structural weakening, despite a limited dynamic response to date.

Overall, our observations indicate a transition toward increased structural vulnerability across the Pine Island Ice Shelf. These findings provide new observational constraints on ice-shelf stability, grounding processes, and transient deceleration mechanisms, with important implications for ice-sheet modeling and future sea-level projections.

How to cite: Chien, Y., Zhou, C., and Riel, B.: Dynamic evolution and emerging structural vulnerability of the Pine Island Ice Shelf, West Antarctica from 2014 to 2025, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4638, https://doi.org/10.5194/egusphere-egu26-4638, 2026.

EGU26-4680 | ECS | PICO | CR2.6

 Temporal evolution and kinematics of a mega-crevasse at Jakobshavn Isbræ revealed by dense GNSS observations 

Anuar Togaibekov, Shfaqat Abbas Khan, Anja Løkkegaard, William Colgan, and Derek Pickell

We analyze the temporal evolution and kinematics of a large mega-crevasse situated in the northern sector of Jakobshavn Isbræ, West Greenland, roughly 50 km north of the glacier’s main flowline. Our study relies on continuous surface-displacement measurements collected by a dense array of 18 permanently operating GNSS stations deployed across and around the crevasse system. These stations recorded ice-surface motion at high temporal resolution over nearly two years, enabling us to capture both seasonal trends and short-term dynamical fluctuations. The resulting displacement time series reveal how strain, opening rates, and relative motion across the crevasse evolved through time, providing new insight into the mechanisms controlling crevasse initiation and growth in this highly dynamic sector of the ice sheet. Fourteen of the GNSS stations are arranged along a profile oriented perpendicular to multiple crevasses, allowing us to quantify both rapid deformation associated with episodic crevasse-opening events and longer-term, seasonally driven variations in crevasse activity linked to meltwater input.Spatial patterns of GNSS-derived velocities show strong tensile strain concentration at crevasse locations, which coincides with the spatial distribution of icequake activities recorded by a colocated array of 18 seismic geophones. We show not only hydrofracture-driven crevasse activities during melt seasons, but also that the presence of mega-crevasses modulates basal sliding velocity by promoting the transfer of surface meltwater to the glacier bed. Our results of field observations provide a foundation for future modeling of crevasse mechanics.

How to cite: Togaibekov, A., Khan, S. A., Løkkegaard, A., Colgan, W., and Pickell, D.:  Temporal evolution and kinematics of a mega-crevasse at Jakobshavn Isbræ revealed by dense GNSS observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4680, https://doi.org/10.5194/egusphere-egu26-4680, 2026.

Abrupt drainage of a proglacial lake provides an opportunity to investigate the response of a lake-terminating glacier to a water level change. In April–July 2020, Lago Greve, a large proglacial lake in the Southern Patagonia Icefield, abruptly drained and the lake level dropped by ~18 m. Using satellite remote sensing data from 2017–2021, we quantified changes in ice velocity, ice-front position, surface elevation, and frontal ablation of three lake-terminating glaciers (Glaciar Pío XI, Greve, and Lautaro), flowing into Lago Greve. The glaciers exhibited contrasting dynamic responses to the same magnitude of water level variation. Glaciar Pío XI decelerated to <10% of the pre-event speed during the drainage, most likely because of decrease in subglacial water pressure. Glaciar Greve showed speed-up, ice-front advance and surface lowering, which were triggered by the reduction in the hydrostatic water pressure acting on the glacier front. Glaciar Lautaro showed no clear response attributable to the drainage. These contrasting behaviors demonstrated the importance of individual settings, e.g., subglacial hydrology, bed geometry, and frontal ablation, to predict the dynamics of calving glaciers, including both lake- and marine-terminating glaciers.

How to cite: Hata, S. and Sugiyama, S.: Dynamic response of three lake-terminating glaciers to an abrupt drainage of Lago Greve, the Southern Patagonia Icefield, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6327, https://doi.org/10.5194/egusphere-egu26-6327, 2026.

EGU26-6553 | PICO | CR2.6

Yearly evolution of Basal Terraces in the cold-cavity of  Ekström Ice Shelf in East Antarctica 

Reinhard Drews, Johannes Noll, Leah-Sophie Muhle, Christian T. Wild, Falk Oraschewski, Olaf Eisen, and Rebecca Schlegel

Basal terraces occur at the base of Antarctic ice shelves. They are characterized by near-vertical walls, often several tens of meters high, which are interconnected by planar, quasi-horizontal, smooth interfaces. Basal terraces have been observed on numerous warm-cavity ice shelves, particularly close to the grounding zone. Their formation has been linked to preferential, ocean-induced horizontal melting at the vertical walls and subdued melting at the horizontal interfaces. Often they are identified as basal melting hot-spot with melt rates much higher than the ice-shelf wide average. However, direct confirmation of these processes on seasonal to yearly timescales do not yet exist.

Here, we present a comprehensive ground-based radar dataset that images the three-dimensional geometry of a basal-terrace field near the grounding zone of the cold-cavity Ekström Ice Shelf. The dataset consists of two time slices spaced one year apart and is analyzed in an Eulerian framework. The radar data are complemented by continuously measuring ApRES thickness measurements, which are integrated into the 3D geometry.

We find that basal melt rates at the horizontal ice face in the nadir direction are approximately one order of magnitude smaller than melt rates inferred from off-nadir reflections, which originate from a nearby inclined interface. All melt rates are with a max of several meters per year small compared to other studies. There is little subseasonal to seasonal variability. Apart from overal thinning, virtually no discernible changes in the 3D geometry are observed over the annual timescale. In airborne radar data, basal terraces occur preferentially near the grounding zone and disappear further seaward.

Taken together, our data support findings from previous studies that ocean-induced melt rates vary significantly over sub-kilometer distances. However, our results also suggest that basal terraces can enter a dormant mode in which they passively advect seaward and maintain a stable geometry without the need for persistently high basal melt rates.

How to cite: Drews, R., Noll, J., Muhle, L.-S., Wild, C. T., Oraschewski, F., Eisen, O., and Schlegel, R.: Yearly evolution of Basal Terraces in the cold-cavity of  Ekström Ice Shelf in East Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6553, https://doi.org/10.5194/egusphere-egu26-6553, 2026.

EGU26-7168 | ECS | PICO | CR2.6

Toward new maps of basal melt rate in grounding zones with tidal flexure from ICESat-2 

Faye Elgart and Brent Minchew

Basal melt rate in the grounding zone is one of the single most important and least-well constrained parameters in modeling the rate and amount of future sea level rise. Sub-ice shelf basal melt rate can be calculated by continuity of mass provided that local ice thickness is well known. However, continent-wide maps of ice thickness that rely on the hydrostatic assumption may underestimate ice thickness near the grounding line. Here, we jointly invert for ice shelf thickness and effective Young’s modulus in the grounding zones of three basins on the Ronne-Filchner Ice Shelf (FRIS or RFIS) based on an elastic beam model of the tidal flexure of ice shelves to make new estimates of basal melt rate in the grounding zone. We show that uncertainty in ice thickness gradient drives uncertainty in the spatial pattern of basal melt rate: adding, eliminating, or moving oceanographic features such as freeze-on bands. This has implications for the set of admissible parameterizations of basal melt rate in models that project the evolution of the Antarctic Ice Sheet in the coming decades and centuries.

How to cite: Elgart, F. and Minchew, B.: Toward new maps of basal melt rate in grounding zones with tidal flexure from ICESat-2, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7168, https://doi.org/10.5194/egusphere-egu26-7168, 2026.

EGU26-8787 | ECS | PICO | CR2.6

 Preliminary reconstruction of deglacial conditions at Ross Bank following the post-LGM collapse of the Ross Bank Ice Rise  

Rachel Meyne, Molly Patterson, Amy Leventer, and Philip Bart

During the post-LGM, the West Antarctic Ice Sheet first retreated from deep-water troughs, followed by retreat from shallower-water banks. Deglacial succession from the troughs show a classic sequence from subglacial sediments deposited below fast-flowing ice streams, that transition upcore to sub-ice-shelf and open-marine sediments accumulated following grounding line and calving front retreat, respectively. Diatom assemblages in these sediments provide powerful evidence for making these environmental interpretations. For example, open-marine facies contain abundant Fragilariopsis curta, a sea-ice associated diatom. In comparison, deglacial successions for bank crests are poorly studied. Understanding bank stratigraphy is important because the formation of an ice rise would influence the pattern of deglaciation. Data acquired during expedition NBP2301/02 demonstrate that the Ross Ice-Shelf (RIS) was formerly pinned to Ross Bank, a broad shallow area in the central Ross Sea. Here, we evaluate the diatom assemblage data from four sediment cores from the shallow-water crest and deep-water flanks of Ross Bank. On the bank crest, the deglacial succession is a sand-rich residual glacial marine deposit. The diatom assemblage contains high to moderate percentages of sea-ice and permanently open-ocean species. These abundances suggests these winnowed products were derived from sediments that initially accumulated in distal sub-ice-shelf and/or open-marine settings. The downcore variations in diatom assemblage and abundance indicate that the intensity of winnowing on the bank was variable after the RIS unpinned. Understanding these processes is important as it can be used to constrain deglacial sequences and to identify reworked intervals in bank-crest core, which when combined with other evidence, can be used reconstruct the pattern and timing of ice shelf unpinning and other clues as to how the local deglacial conditions evolved.

How to cite: Meyne, R., Patterson, M., Leventer, A., and Bart, P.:  Preliminary reconstruction of deglacial conditions at Ross Bank following the post-LGM collapse of the Ross Bank Ice Rise , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8787, https://doi.org/10.5194/egusphere-egu26-8787, 2026.

EGU26-10022 | ECS | PICO | CR2.6

Understanding Ice Sheet Instability: A Review of Thermodynamic and Mechanical Drivers Behind Mass Loss 

Dilan Kılınçoğlu, İsmail Ömer Yılmaz, Bülent Gültekin Akınoğlu, and Abdullah Buğrahan Karaveli

The rapid melting of polar ice sheets is one of the biggest unknowns in sea-level-rise models. The instability is not due to a single factor but emerges due to the complex coupling of thermodynamic forcing and mechanical response. This paper provided a review of the physical mechanisms governing these processes with an emphasis on the transition from surface melt to structural failure.

The authors analyze surface energy balance and latent heat release from the firn-ice aquifers instability in the ice sheet. We also investigate how these thermal anomalies become mechanical drivers, such as hydro-fracturing and basal lubrication, that reduce effective stress and accelerate ice flow. The link between Marine Ice Sheet Instability (MISI) hypothesis and purely atmospheric forcing is also discussed from continuum mechanics perspective.

By reviewing the existing literature through a physics view, this paper wants to identify the gaps in the current ice sheet models (ISM) in terms of stress transmission and fracture propagation parameterization. The purpose of this project is to lay the theoretical groundwork for a master’s thesis that aims to use a more integrated model of the non-linear response of ice sheets to climate warming.

How to cite: Kılınçoğlu, D., Yılmaz, İ. Ö., Akınoğlu, B. G., and Karaveli, A. B.: Understanding Ice Sheet Instability: A Review of Thermodynamic and Mechanical Drivers Behind Mass Loss, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10022, https://doi.org/10.5194/egusphere-egu26-10022, 2026.

Marine-terminating glaciers in Arctic fjords exhibit complex and highly variable calving behavior, reflecting interactions between ice dynamics and fjord processes. Better understanding of calving is required for accurate prediction of ice loss, ocean freshening and sea level rise. Here, we study calving at seven marine-terminating glaciers in Hornsund Fjord, Svalbard over the period 2015 – 2022. To do so, we use combination of remote sensing products for glacier positions and dynamics, and measurements of other environmental parameters. We investigate the temporal variability of calving at seasonal and annual timescales, including the winter months which are usually not considered. Furthermore, we also study the spatial variability of calving along the glacier width, which further reveals small scale features on the termini related to different calving styles. Together, this work highlights the variable nature of calving across different glaciers within a single fjord.

How to cite: Maniktala, D. and Glowacki, O.: Glacier Calving in Hornsund Fjord, Svalbard: Spatio-Temporal Variability, Terminus Geometry, and Environmental Drivers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11616, https://doi.org/10.5194/egusphere-egu26-11616, 2026.

EGU26-12502 | PICO | CR2.6

Historical Calibration of Basal Melt Parameters in a circum-Antarctica Ice-Sheet Model 

Qing Qin, Jan De Rydt, Vio Coulon, and Frank Pattyn

The Antarctic Ice Sheet (AIS) is a major contributor to future global sea level rise. Approximately half of the surface mass gain is offset by ocean-induced basal melting, highlighting the critical role of ice-ocean interactions. Uncertainty in projections of AIS evolution remains strongly linked to how basal melting is represented and calibrated in ice-sheet models, together with divergent future climate forcing scenarios.

In this study, we use a circum-Antarctic high-resolution configuration of the Úa ice-sheet model to conduct a series of 360 hindcast simulations (spanning 2000-2020) to quantify uncertainties and sensitivities in modelled ice-shelf melt. The ensemble covers a range of ice rheology and basal sliding parameters, as well as multiple basal melt parameterizations (quadratic, PICO and plume) and a physically plausible range of parameter choices for each parameterization.

Whereas previous studies have calibrated basal melt parameters using fixed ice-sheet geometries or relied primarily on basal melt observations alone, this study presents two advances: 1) ice-ocean feedbacks were included in the calibration through temporally evolving basal melt rates, and 2) simulated changes in ice velocity and thickness over the hindcast period were validated against remote-sensing data.

After calibration, model performance improves in the representation of both basal melt rates and ice-dynamic response patterns. For most basal melt parameters, the posterior distributions exhibit clear localization relative to the prior, indicating well-defined optimal parameter values. The resulting calibrated parameter ranges therefore provide a more robust foundation for future long-term projections of AIS evolution and its contribution to global sea-level rise. Notably, these optimal parameter values differ from those obtained using calibration approaches based on fixed ice-shelf cavities or basal-melt observations alone. We also examine regional variability in calibration results. The relative performance of basal melt parameterizations differs between Antarctic sectors, while optimal parameter ranges within each parameterization remain broadly consistent with the Antarctic-wide calibration.

How to cite: Qin, Q., Rydt, J. D., Coulon, V., and Pattyn, F.: Historical Calibration of Basal Melt Parameters in a circum-Antarctica Ice-Sheet Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12502, https://doi.org/10.5194/egusphere-egu26-12502, 2026.

EGU26-12974 | ECS | PICO | CR2.6

Modeling frontal ablation in global glacier models (Joint Bayesian) 

Ruitang Yang, Lizz Ultee, Kristoffer Aalstad, Matvey Debolskiy, Regine Hock, Patrick Schmitt, David Rounce, and Tian Li

Accurate estimation of frontal ablation of water‑terminating glaciers is essential for assessing global glacier mass change and projecting sea‑level rise. We present a hybrid framework that couples a SERMeQ‑based frontal‑ablation component with climatic mass‑balance from PyGEM and ice dynamics from OGGM, and we introduce an adaptive particle‑batch smoother to jointly calibrate all model parameters simultaneously. The model simulates centreline length change and mass‑balance components at monthly resolution and updates flow‑line geometry accordingly. Calibration assimilates both decadal averaged geodetic mass‑balance estimates and remote‑sensing annual timeseries terminus‑position changes, constraining the coupled dynamics and ablation processes within a single, physically consistent framework. Applied regionally to 71 tidewater glaciers in Svalbard, the framework reproduces observed seasonal behaviour and hindcasts, while providing improved projections of future glacier evolution. These results offer more robust regional estimates of contributions to sea‑level rise and freshwater availability and identify priorities for further reducing uncertainties in frontal‑ablation estimates.

How to cite: Yang, R., Ultee, L., Aalstad, K., Debolskiy, M., Hock, R., Schmitt, P., Rounce, D., and Li, T.: Modeling frontal ablation in global glacier models (Joint Bayesian), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12974, https://doi.org/10.5194/egusphere-egu26-12974, 2026.

EGU26-13590 | ECS | PICO | CR2.6

Inferring basal melt rates underneath the Ross Ice Shelf using data assimilation 

Max Brils and Hilmar Gudmundsson

More than 80% of the grounded ice of the Antarctic ice sheet drains into the ocean through ice shelves. Loss of these ice shelves could cause an increase of the discharge of grounded ice which would lead to additional sea-level rise. Roughly half of the ice shelves’ mass is eventually lost through melting from the underside, where the ice gets in contact with warmer ocean waters. However, estimating these basal melt rates is notoriously difficult. Here, we present a novel methodology for calculating the melt rates by assimilating remotely derived estimates of surface velocities, ice sheet thickness, surface elevation changes and modelled surface mass balance using an ice sheet model (Úa). This methodology allows for a less noisy, physically consistent estimate of the ice mass divergence, and weighs each of the input data with their uncertainty. As a case study, we apply our method to the Ross ice shelf and find that the melt rates are highly spatially variable.

How to cite: Brils, M. and Gudmundsson, H.: Inferring basal melt rates underneath the Ross Ice Shelf using data assimilation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13590, https://doi.org/10.5194/egusphere-egu26-13590, 2026.

EGU26-15645 | ECS | PICO | CR2.6

Implications of realistic Antarctic ice shelf basal melting during 2006–2016 on Southern Ocean climate 

Zhu Zhu, Jiping Liu, Yan Liu, Torge Martin, Mirong Song, Chao-Yuan Yang, Wenmi Chai, and Qinghua Yang

Antarctic ice shelves have been losing mass at an increasing rate in recent decades. This process is missed in most climate models. Recent studies added extra freshwater along the Antarctic coast to investigate its potential effects. However, these studies used either model simulated or uniformly distributed freshwater inputs, so that climate impacts of realistic, time- and space-varying meltwater remain uncertain. Here, we investigate implications of the recent change in basal melt rates from 93 Antarctic ice shelves from the 1990s to 2006–2016 (223 Gt yr-1 on average) on Southern Ocean climate using a fully coupled model. The most prominent response is significant increased sea ice coverage in the northern Amundsen Sea and decreased sea ice coverage in the northern Weddell Sea. The northern Amundsen Sea experiences sea surface and near-surface atmospheric cooling and a strengthened Amundsen Sea Low, while the northern Weddell Sea exhibits warming and above-normal sea-level pressure. In the Amundsen Sea, both oceanic thermodynamic and atmospheric dynamical effects contribute to sea ice growth during the freeze-up season, with atmospheric dynamics playing a dominant role during the melting season. In contrast, sea ice decline in the Weddell Sea is primarily driven by oceanic warming during the freeze-up season and atmospheric circulation anomalies during the melting season. Our results highlight the critical role of atmospheric circulation changes in shaping the contrasting sea-ice and temperature responses in the Amundsen and Weddell Seas and underscore the importance of representing realistic ice-shelf basal melt in coupled climate models to better understand Southern Ocean climate variability.

How to cite: Zhu, Z., Liu, J., Liu, Y., Martin, T., Song, M., Yang, C.-Y., Chai, W., and Yang, Q.: Implications of realistic Antarctic ice shelf basal melting during 2006–2016 on Southern Ocean climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15645, https://doi.org/10.5194/egusphere-egu26-15645, 2026.

EGU26-17895 | PICO | CR2.6 | Highlight

Evolution of the Northeast Greenland glaciers in a warming world 

Claudia Wekerle, Michael Wolovick, Yuting Dong, Martin Rückamp, Ralph Timmermann, and Torsten Kanzow

The Northeast Greenland Ice Stream (NEGIS) drains through two major outlet glaciers: the 79 North Glacier (79NG) and Zachariae Isstrøm (ZI). Since the 2000s, these glaciers have exhibited contrasting behavior: while the ZI ice shelf has retreated dramatically and transitioned to a tidewater glacier, the 79NG ice tongue has remained relatively stable in extent despite significant thinning. The retreat and thinning of both glaciers have accelerated the upstream ice stream, with important implications for global sea level rise.

We present a novel coupled model that integrates the Ice-sheet and Sea-level System Model (ISSM) with the Finite volumE Sea Ice-Ocean Model version 2 (FESOM2). The ice sheet model domain encompasses the NEGIS region, while the global ocean model features enhanced mesh resolution on the Northeast Greenland continental shelf and explicitly resolves the ice shelf cavities of both 79NG and ZI. This coupling enables dynamic representation of ice sheet-ocean-sea ice interactions, including grounding line migration and ice geometry evolution.

A hindcast simulation spanning 2008-2023, forced by atmospheric reanalysis data, reproduces the observed calving front retreat at ZI with good fidelity, validating our modeling approach. Beyond validation, this experiment reveals that the rapid ZI retreat is driven primarily by internal ice dynamics rather than changes in oceanic forcing. We extend our analysis through climate projection simulations using atmospheric forcing from CMIP6 scenarios. Applying both low and high emission scenarios (SSP126 and SSP585), we are able to  assess the possible future evolution of these glaciers until the end of this century.



How to cite: Wekerle, C., Wolovick, M., Dong, Y., Rückamp, M., Timmermann, R., and Kanzow, T.: Evolution of the Northeast Greenland glaciers in a warming world, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17895, https://doi.org/10.5194/egusphere-egu26-17895, 2026.

EGU26-19807 | PICO | CR2.6

Multi-decadal ice shelf retreat driven by ocean wave erosion in the absence of sea-ice 

Bertie Miles, Anna Crawford, and Nick Homer

In recent years, a number of studies have focused on the mechanical impacts of sea-ice loss on Antarctic ice shelves. These impacts arise either through the potential buttressing provided by multi-year landfast sea ice or through increased ocean swell as pack ice diminishes. Increasing periods of sea-ice-free conditions near ice shelves also modify thermal forcing, as sea-surface temperatures seasonally increase. The number of sea-ice-free days has increased by around 50% at the eastern Getz Ice Shelf since the 1970s, to the point where it is virtually sea-ice-free throughout December and January each year, when solar insolation is at its highest. With the exception of the Ross Ice Shelf, no other major ice shelf experiences comparable summer sea-ice-free conditions. We explore the calving processes along the eastern Getz Ice Shelf, with the underlying hypothesis that these processes will become increasingly relevant across Antarctica as sea ice continues to diminish.

The calving fronts of the eastern outlets of the Getz Ice Shelf have been retreating since the earliest satellite observations in the 1970s. This retreat is persistent and is characterised by advance during the winter months and retreat during the summer, with frontal ablation rates of around 650 m a⁻¹. This retreat has occurred despite no detectable changes in ice-shelf damage over the past 50 years, the absence of landfast sea ice, limited changes in ice velocity seaward of the grounding zone, and no recorded thinning in the outlet experiencing the most significant retreat. Surface profiles of the ice shelf reveal widespread evidence of rampart–moat structures, which are highly indicative of buoyancy-driven calving. Sea-ice-free conditions allow the ocean surface to heat up; this heat is sufficient to drive undercutting at the ice front, resulting in cliff retreat and the formation of an underwater foot, which in turn promotes buoyancy-driven calving, termed ‘footloose’ calving. In the case of the easternmost outlet of the Getz Ice Shelf, retreat is already progressing into its embayment; in the coming years, this will result in a loss of buttressing, acceleration, and a change in the dynamic state of the ice shelf.

Nearly all other Antarctic ice shelves remain encased by sea ice during the summer. Many of these ice shelves, particularly those in regions such as Dronning Maud Land, flow at only ~200 m a⁻¹, meaning that a similar  frontal ablation rate of 650 m a⁻¹ would be highly significant. As sea ice diminishes and this mechanism becomes increasingly important, we cannot rule out widespread retreat of Antarctica’s ice shelves driven by a process not currently incorporated into ice-sheet models.

How to cite: Miles, B., Crawford, A., and Homer, N.: Multi-decadal ice shelf retreat driven by ocean wave erosion in the absence of sea-ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19807, https://doi.org/10.5194/egusphere-egu26-19807, 2026.

EGU26-2284 | ECS | Posters on site | GM9.3

Ice shelf retreat decouples Piglet Glacier from the Pine Island catchment and amplifies dynamic mass loss 

Byeong-Hoon Kim, Changhyun Choi, Choon-Ki Lee, Ki-Weon Seo, Won Sang Lee, Ji Sung Na, Sukyung Yoon, Clare Eayrs, Bemjamin Wallis, Anna Hogg, Hamish Pritchard, and Pierre Dutrieux

Piglet Glacier, formed by ~20% area loss of the Pine Island Ice Shelf in 2017-2020, provides a compact analogue for testing how ice‑shelf damage and retreat alters inland glacier dynamics and drainage-basin mass balance. We use Sentinel‑1 feature‑tracking (October 2014~) and CryoSat‑2 (July 2010~) interferometric swath altimetry to monitor change on Piglet Glacier through to May 2025, quantifying both the propagation of ice speedup and the thickness change response. Relative to a 2015-2017 baseline, speed near the grounding line increased by ~40%, with acceleration propagating ~50 km inland with no resolvable lag, indicating efficient transmission of reduced buttressing into grounded ice. Firn‑corrected altimetry reveals a concurrent intensification of dynamic thinning: the basin‑integrated dynamic volume‑loss rate rose from ~2.9 to ~4.5 km3 yr-1 (a 60% increase). Downstream, post‑calving acceleration was concentrated along pre‑damaged shear margins, and subsequent loss of shear‑margin mélange in 2024-2025 promoted further mechanical decoupling. Sustained shear‑margin attrition and frontal retreat are fragmenting the Pine Island basin system and accelerating mass loss from Piglet Glacier. This example provides a tractable benchmark for improving projections of West Antarctica’s near‑term sea‑level contribution. Future modelling studies should include shear‑margin damage, tributary detachment, and rapid inland transmission of buttressing loss, to improve process‑level constraints.

How to cite: Kim, B.-H., Choi, C., Lee, C.-K., Seo, K.-W., Lee, W. S., Na, J. S., Yoon, S., Eayrs, C., Wallis, B., Hogg, A., Pritchard, H., and Dutrieux, P.: Ice shelf retreat decouples Piglet Glacier from the Pine Island catchment and amplifies dynamic mass loss, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2284, https://doi.org/10.5194/egusphere-egu26-2284, 2026.

Low-lying deltaic regions across the world are increasingly transforming into “sinking landscapes” under the combined influence of sea-level rise, land subsidence, cryosphere change, and intensifying hydro-climatic extremes. This study examines human resilience in Arctic and Asian deltas through a comparative assessment of adaptive capacities, with a detailed case study from the Indian Sundarbans, one of the most climate-exposed mangrove delta systems globally. Although Arctic deltas and Asian tropical deltas differ markedly in climate, geomorphology, and socio-economic context, both are experiencing accelerated environmental change that threatens livelihoods, settlements, and ecosystem stability.

The research adopts an integrated socio-hydrological framework, combining geospatial analysis, secondary climate and hydrological datasets, and community-level vulnerability indicators. Arctic delta regions are analysed in terms of permafrost thaw, coastal erosion, and diminishing sea-ice protection, while the Sundarbans case highlights subsidence, cyclonic storm surges, tidal flooding, salinity intrusion, and sediment deprivation. In the Sundarbans, adaptive capacity is assessed through livelihood diversification (fishing, forest-based activities, and eco-tourism), seasonal and distress migration, mangrove-dependent ecosystem services, and community-based disaster risk reduction mechanisms.

Comparative analysis reveals parallel vulnerability pathways across Arctic and Asian deltas, including high dependence on natural resources, limited infrastructure, and governance challenges that constrain long-term adaptation. However, distinct adaptation strategies emerge. Arctic communities exhibit resilience through mobility, flexible settlement patterns, and indigenous ecological knowledge, while Sundarbans communities rely on ecosystem-based adaptation, collective coping practices, and incremental livelihood adjustments. Despite these strategies, both contexts face limits to adaptation as environmental change outpaces institutional and economic support systems.

The findings underscore that resilience in sinking landscapes is not solely determined by physical or technological interventions but is deeply embedded in social relations, cultural practices, and access to environmental resources. By foregrounding the Sundarbans as a representative Asian delta case, this study contributes to a comparative understanding of human adaptation across climatic extremes. The research offers policy-relevant insights for sustainable delta management, climate adaptation planning, and climate justice, emphasizing the need for locally grounded yet globally informed strategies to enhance resilience in vulnerable deltaic futures.

Keywords: Human resilience; Adaptive capacity; Sinking landscapes; Sundarbans delta; Arctic deltas; Socio-hydrology; Climate change adaptation; Delta vulnerability; Ecosystem-based adaptation

How to cite: Laha Salui, C.: Human Resilience in Sinking Landscapes: Comparing Adaptive Capacities across Arctic and Asian Deltas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3296, https://doi.org/10.5194/egusphere-egu26-3296, 2026.

EGU26-4165 | Orals | GM9.3

Geomorphic and climatic controls on moraine building and preservation in the Southern Alps Kā Tiritiri o te Moana 

Ann Rowan, Karlijn Ploeg, David Egholm, Chris Clark, Vivi Pedersen, Stephanie Mills, and Tim Barrows

Glacier margins fluctuate in response to climate change and often record these changes in the landscape by building ice-marginal (terminal and lateral) moraines. Glacial landscapes are therefore a potentially valuable archive of terrestrial palaeoclimate change. Typically a cooling climate causes glaciers to expand and warming causes glaciers to shrink. However, the dynamic glacier response time and the influence of high-relief mountainous topography on glacier dynamics complicates this behaviour, such that ice-marginal moraines are not always a straightforward record of palaeoglacier or palaeoclimate change. In tectonically active landscapes, such as the Southern Alps Kā Tiritiri o te Moana of Aotearoa New Zealand, high rates of hillslope erosion deliver large volumes of sediment to glaciers, leading to the formation of supraglacial debris layers that further decouple glacier behaviour from climate change.

We use the higher-order ice-flow model iSOSIA to simulate changes in erosion, ice extent and thickness in the response to Late Quaternary climate change and the resulting formation and preservation of moraines in a synthetic mountainous landscape. Our results show that the rate of palaeoclimate change relative to a glacier’s response time determines the geometry, number, and position of ice-marginal moraines, that glaciers can build distinct moraines in the absence of climate change, and that the distance from the glacial maximum may not represent the chronological order of moraine formation. While moraines can be preserved despite erosion by various surface processes and by being overrun during subsequent glaciations, moraine sequences frequently contain gaps that could be misinterpreted as representing periods of climate stability. We apply this model to Franz Josef Glacier Ka Roimata o Hine Hukatere to reconstruct glacier evolution and moraine building in the Southern Alps Kā Tiritiri o te Moana during the Last Glacial Maximum and subsequent deglaciation.

How to cite: Rowan, A., Ploeg, K., Egholm, D., Clark, C., Pedersen, V., Mills, S., and Barrows, T.: Geomorphic and climatic controls on moraine building and preservation in the Southern Alps Kā Tiritiri o te Moana, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4165, https://doi.org/10.5194/egusphere-egu26-4165, 2026.

EGU26-5783 | Orals | GM9.3

Using 137Cs measurements to detect changes in sedimentation rates in a floodplain area of northern Norway. Preliminary results of a field sampling campaign 

Paolo Porto, Michal Habel, Halina Kaczmarek, Monika Szymańska-Walkiewicz, and Marta Brzezińska

Floodplain sediment records may provide important information on soil erosion and deposition rates over large catchments and for different time windows. In this context, the use of anthropogenic and geogenic radiotracers has recently attracted increasing attention for their ability to act as sediment markers and to reflect the environmental impacts due to variation in land use and recent climate changes. 137Cs is one of the most employed radiotracers for sediment chronology due to its easy detectability in the environment and to its strong ability to be retained by sediments in depositional areas. 137Cs activity in sediments reflects the temporal fallout occurred in the area and, as such, it proved to be a very effective indicator to reconstruct the trend of soil erosion and sedimentation rates during the last 6-7 decades. In this contribution, a floodplain area in northern Norway was identified as a ‘pilot site’ to explore possible anthropogenic impacts and climate change effects on deposition rates from uncultivated sites. Sediment cores collected in the area were analysed for 137Cs content and provided evidence of Chernobyl fallout. This result made it possible to obtain information on sedimentation rates for different time windows (i.e. 1963-1986 and 1986-2024) and suggested an increase of sedimentation rates during the last 4 decades.

How to cite: Porto, P., Habel, M., Kaczmarek, H., Szymańska-Walkiewicz, M., and Brzezińska, M.: Using 137Cs measurements to detect changes in sedimentation rates in a floodplain area of northern Norway. Preliminary results of a field sampling campaign, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5783, https://doi.org/10.5194/egusphere-egu26-5783, 2026.

EGU26-6893 | ECS | Posters on site | GM9.3

Correlating contributors to glacial morphometric signatures in the DEM topography of the European Alps’ crystalline massifs 

Isabel Wapenhans, Peter van der Beek, Pierre Valla, and Xavier Robert

Repeated extensive Pleistocene glaciations of the European Alps have imposed a spatially heterogeneous imprint on Alpine topography. Physics-based frameworks of glacial erosion at the catchment scale explain prominent overdeepened topography in some areas, but mixed or subdued topographic signatures in others, with differences in coupled climatic, surface, and lithospheric factors that enhance or modulate glacial erosion potential. Yet, systematic orogen-scale connections between input glacial forcings and resultant observable morphometric features remain limited, and the spatial heterogeneity of glacial topographic reshaping remains poorly understood.

We target the prominently glaciated crystalline massifs of the Eastern (Hohe Tauern) and Central (Aar) and Western (Mont Blanc) Alps, which share rapid Neogene exhumation, resistant lithologies, and high local relief, yet exhibit intra-massif morphometric contrasts: steep, glacially overdeepened valleys adjacent to less glacially modified catchments. Our comparison addresses two key questions: Why do certain areas display more pronounced glacial reshaping than others despite widespread Last Glacial Maximum ice coverage? Which forcings (climatic, geodynamic etc.) dominate the development of end-member glacial morphometries, and do these inputs vary between and within the studied massifs?

We derive classical topographic and valley specific metrics from the ESA Copernicus 30-m resolution DEM using established geospatial tools, treating them as measurable landscape metrics. We use random forest regression analysis, drawing on model-derived glacial indicators, landscape-derived variables, modern uplift rates and time-integrated measurements such as exhumation and catchment-wide denudation rates, to identify the strongest predictors of glacial signatures.

Preliminary results underscore the interplay of geodynamic preconditioning and climatic modulation in generating distinct glacial fingerprints. This aligns with the findings of a suite of Alpine site-specific works using thermochronology, cosmogenic nuclides, and numerical modeling to investigate similar questions at a local scale, where these factors are spatially more uniform. Our ongoing work refines the statistical framework outlined and tests for possible process feedbacks. Advancing an orogen-scale understanding of climate-tectonic interactions in mountain landscape evolution can aid our understanding of the implications for sediment fluxes, geohazards, and ecological responses in mountain enviroments.

How to cite: Wapenhans, I., van der Beek, P., Valla, P., and Robert, X.: Correlating contributors to glacial morphometric signatures in the DEM topography of the European Alps’ crystalline massifs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6893, https://doi.org/10.5194/egusphere-egu26-6893, 2026.

EGU26-7365 | ECS | Orals | GM9.3

Global patterns of stable isotope signatures across cryosphere and hydrological components of glacierized catchments 

Edison Edu Jara Tarazona, Melanie Vital, Andrew Wade, Janie Masse-Dufresne, Aurel Persoiu, Marjan Temovski, Luzmilla Dàvila Roller, Francisco Fernandoy, Jeonghoon Lee, Bakhriddin Nishonov, Edson Ramirez, Zarina Saidaliyeva, Maria Shahgedanova, Pu Tao, Polona Vreca, and Yuliya Vystavna

Glacierized catchments play an important role in regional and global water resources by storing, releasing, and redistributing freshwater. Stable water isotopes (SWI, δ¹⁸O and δ²H) are widely used to trace these processes, providing information on moisture sources, elevation and temperature effects, subsurface storage, and mixing between cryosphere and non-cryosphere components. They also allow quantifying the contributions of the cryosphere and hydrological component to the streamflow. Integrating SWI analysis into studies of glacierized catchments helps better quantify glacier contributions to regional water resources and assess how these contributions change under different climate conditions. 

Despite decades of isotope-based studies in glacierized environments, SWI data remain fragmented across regions and hydrological components. In this study, we introduce the first global, harmonized database of SWI signatures from cryosphere and hydrological components in glacierized catchments, enabling a global synthesis of isotope patterns. The database compiles 12,348 isotope records from peer-reviewed literature, institutional repositories, and public data platforms published between 1960 and 2025. It integrates δ¹⁸O, δ²H, and derived d-excess values for a wide range of hydrological endmembers, including precipitation, snow, stream, groundwater, lake, snowpack, snowpack melt, glacier ice, glacier meltwater, supraglacial meltwater, firn, ice-cored moraines, talus slopes, rock glacier and permafrost thaw. Each record is georeferenced and accompanied by standardized metadata describing sampling context, elevation, temporal coverage, analytical method, and uncertainty. This database covers five continents and 20 countries, with the highest data density in the Himalaya–Tibet region. The database focuses on continental glacierized catchments where glaciers interact directly with surface waters and groundwater, excluding Greenland and Antarctic ice sheets due to their specific hydrological conditions.  

The comparative analysis of isotope distributions reveals systematic contrasts among endmembers and continents. At the global scale, δ¹⁸O values (‰ VSMOW2) clearly distinguish cryosphere and hydrological endmembers. Continental-scale patterns of δ¹⁸O highlight the dominant influence of temperature, elevation, atmospheric circulation, and moisture source on isotope variability. North America shows the widest isotopic range due to strong latitude and elevational contrasts. Snow and glacier waters in the Andes are strongly depleted (−18 to −14‰) reflecting orographic effects. African data are limited but indicate warm conditions and evaporative enrichment, while Asia shows large variability driven by strong climatic and topographic gradients. European waters exhibit moderate depletion typical of mid-latitude precipitation regimes. Distributions of d-excess provide information on moisture sources and post-depositional processes. Most samples show positive d-excess values (8–15‰), indicating that the primary atmospheric signal is preserved. 

Overall, this dataset aims to support the applications of isotope tracers in water resource studies a provides benchmark constraints for isotope-enabled hydrological models (e.g., iCESM, IsoHydro, JAMS200). The interpretations presented here represent an initial exploration of this unique global compilation. By making these data openly available, we aim to support more detailed investigations into the processes governing the hydrology of glacierized catchments.

How to cite: Jara Tarazona, E. E., Vital, M., Wade, A., Masse-Dufresne, J., Persoiu, A., Temovski, M., Dàvila Roller, L., Fernandoy, F., Lee, J., Nishonov, B., Ramirez, E., Saidaliyeva, Z., Shahgedanova, M., Tao, P., Vreca, P., and Vystavna, Y.: Global patterns of stable isotope signatures across cryosphere and hydrological components of glacierized catchments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7365, https://doi.org/10.5194/egusphere-egu26-7365, 2026.

EGU26-10724 | ECS | Posters on site | GM9.3

Application of backscatter time-series analysis and offset tracking for the identification of glacier surges on Svalbard 

Mirosław Czyżewski, Michał Tympalski, Marek Sompolski, and Wojciech Milczarek

The study of glacier surges, which involve periodic increases in flow velocity even to several orders of magnitude, is crucial for a better understanding of glacier dynamics in Arctic regions. Knowledge of the causes, course, and mechanisms of this phenomenon can help determine the role of glaciers as indicators of global climate change. It is also very important for safety and risk management reasons. A relatively new method of studying glacial surges is the analysis of backscatter changes in SAR images, which indicate deformations and variable properties of the glacier surface during the active phase. However, unambiguous identification of the phenomenon requires analysis of changes in the surface velocity of the glacier.

In this study we analyze a time series of Sentinel-1 mission data for Svalbard for the years 2016-2025 to track the long-term dynamics of glaciers. We detect backscatter anomalies that can be associated with surge activity. We then compare the results with surface velocity data obtained by offset tracking on SAR imagery. Based on the results, we conclude that the two methods are complementary. The methodology used can be applied in further studies of glacier surges and expand the knowledge of surge mechanisms that are not yet fully understood. 

How to cite: Czyżewski, M., Tympalski, M., Sompolski, M., and Milczarek, W.: Application of backscatter time-series analysis and offset tracking for the identification of glacier surges on Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10724, https://doi.org/10.5194/egusphere-egu26-10724, 2026.

EGU26-10994 | Orals | GM9.3

Disappearing glaciers and emerging landscapes: new opportunities or rising risks? 

Sara Savi, Ananya Pandey, Bodo Bookhagen, Francesca Mura, Andrea Andreoli, and Francesco Comiti

Global warming has a major impact on the cryosphere. Mountains worldwide are witnessing the inexorable loss of glaciers, the degradation of permafrost, and a growing frequency of droughts and extreme precipitation events. Whereas many eyes are pointed to the loss of beauty, biodiversity, and freshwater resources, as well as to the catastrophic collapses of mountain slopes around the globe, only little attention is deserved to the new emerging post-glacial landscapes. A narrow belt of land remains bare for the time required to vegetation to adapt and migrate to higher elevations. This bare land is often characterized by fine sand and big boulders, unconsolidated debris, and over-steepened slopes that easily become unstable and can generate large amount of sediment which, if mobilized, may threaten the downstream valleys.

The paraglacial adjustment may require hundreds of years to reach equilibrium. In the classical model, the peak of sediment yield is expected to come immediately after the onset of the deglaciation, to then gradually decline towards a long-term equilibrium. Yet, climatic or anthropogenic perturbations can significantly modify the expected decline in sediment yield over time. Increased frequency of extreme precipitation events, associated with shifts in snowfall cover and with the increase of unconsolidated sediment, may create unprecedented conditions where enormous amount of sediment may be available to be mobilized and transported to the valley bottoms. Quantifying these volumes, and especially understanding the peaks around the expected sediment-transport curve, is fundamental for the communities living in high mountain areas, for river system management, and for the mitigation of risks associated with debris-flood events. In this context, it becomes essential to understand: 1) where are we along the paraglacial adjustment curve, and especially, 2) what frequency and intensity should be expected for the climate-induced peaks in sediment yield.

In the Sulden/Solda catchment (South Tirol, Italy) ongoing investigations aim to address these questions. New cosmogenic data allows to estimate average sediment production over centennial timescales, whereas modern digital elevation models allow to quantify recent average values. Interestingly, preliminary data indicates that long-term and modern averages are very similar, rising a new set of questions rather than answering those posed above. Are we still on the rising limb of the paraglacial curve? Or did sediment yield decline and are we witnessing the effects of global warming? And how do extreme precipitation events enter in the picture? Hopefully, by May, some of these questions will have been answered, and it will be a pleasure to discuss them at EGU.

How to cite: Savi, S., Pandey, A., Bookhagen, B., Mura, F., Andreoli, A., and Comiti, F.: Disappearing glaciers and emerging landscapes: new opportunities or rising risks?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10994, https://doi.org/10.5194/egusphere-egu26-10994, 2026.

Glaciological research has demonstrated that mechanisms such as fracturing, faulting, and foliation play a fundamental role in controlling ice flow patterns, debris entrainment, and styles of glacier retreat across diverse dynamic settings. While these relationships are well-documented for High-Arctic polythermal and cold-based glaciers, and increasingly for marine-terminating systems, the structural evolution of active temperate valley glaciers remains comparatively understudied. This study addresses this gap through an investigation of Sandfellsjökull, an active temperate outlet of Mýrdalsjökull Ice Cap. Previous research at Sandfellsjökull has focused primarily on proglacial geomorphology, leaving the evolution of its internal structure and margin dynamics largely unconstrained. Here, a multi-method approach is applied to quantify surface and sub-surface characteristics, combining geospatial photogrammetric analysis of historical aerial orthophotographs, UAV-derived imagery, ITS_LIVE (Inter-mission Time Series of Land Ice Velocity and Elevation) products and digital elevation models (e.g., ÍslandsDEM v1.0) with detailed ice facies, structural, and sedimentological analyses at the glacier margin. These datasets are used to develop a conceptual model of structural evolution between 1945 and 2025 and to assess the influence of bedrock topography on deformation patterns and debris entrainment.

Preliminary results reveal pronounced lateral and down-glacier variability in structure and debris distribution. The southern margin exhibits longitudinal compressional crevassing and confined ice flow between bedrock outcrops, with supraglacial meltwater channels cross-cutting debris cones and feeding an active outwash system. In contrast, the northern margin is characterised by a concentric tephra band deforming around an undercut bedrock step and transitioning abruptly into stagnant, debris-covered ice undergoing passive downwasting. Stratigraphic analyses from 12 sections indicate a dominant dispersed ice facies with stratified debris bands entraining fine-grained tephra - likely derived from the 1918 Katla eruption - as well as angular basaltic lithologies derived from freshly plucked bedrock. These observations highlight the critical role of topography in governing glacier structure, debris entrainment, and retreat style, with implications for basal ice formation (regelation and glaciohydraulic supercooling) on adverse slopes. Ongoing work in this study integrates structural mapping with changes in fracture density, surface elevation and velocity, as well as meteorological data, to resolve the spatio-temporal evolution of Sandfellsjökull in the context of recent climate warming.

How to cite: Gath, M., J A Evans, D., Jamieson, S., and Guild, A.: Structural evolution of an actively retreating glacier (1945 - 2025) modulated by bedrock steps and terminal overdeepening: Sandfellsjökull, east Mýrdalsjökull, Iceland., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13879, https://doi.org/10.5194/egusphere-egu26-13879, 2026.

EGU26-15188 | Orals | GM9.3

Transient hydrosystems in deglaciating subarctic catchments: insights from a decade of research in the St. Elias Mountain Green Belt 

Michel Baraer, Bastien Charonnat, Éole Valence, Adam Tjoelker, Jeff McKenzie, Janie Masse-Dufresne, Adrien Dimech, and Bryan Mark

Rapid cryosphere degradation is profoundly transforming hydrological processes in glacierized catchments worldwide. In subarctic environments, glacier retreat progressively reduces the direct contribution of ice melt to streamflow, while other cryospheric and periglacial components become increasingly influential, often in transient and non-linear ways. In particular, permafrost thaw and the reorganization of periglacial landscapes give rise to new, evolving pathways for water storage and transfer.

Over the past decade, we have examined these dynamics in the Shä́r Ndü Chù Duke River watershed, located within Kluane First Nation territory in the St. Elias Mountain Green Belt. Long-term observations reveal that the various cryospheric components of deglaciating valleys respond at different rates, leading to asynchronous shifts in hydrological and hydrogeological processes. As a result, the watershed functions as a continuously evolving hydrosystem rather than progressing toward a single, stable post-glacial state.

Our investigation combines ground-based and drone-borne geophysical surveys, thermal infrared and LiDAR observations, hydrometeorological monitoring, and hydrochemical tracers to characterize both surface and subsurface processes. These complementary methods highlight the growing role of groundwater in watershed outflows, driven by the widespread development of debris-covered and buried ice and by the mantling of formerly glacierized terrain. Such conditions modify surface energy exchanges and promote a transition from relatively direct surface runoff to enhanced infiltration and complex subsurface drainage networks.

Dynamic periglacial landforms, including rock glaciers containing long-lived debris-insulated ice, further disrupt surface–groundwater connectivity and redistribute flow paths across the landscape. Although debris cover slows the degradation of buried ice and permafrost relative to exposed ice, continued cryospheric loss remains inevitable. Collectively, our results demonstrate that hydrological routing in deglaciating subarctic catchments is highly transient, with important implications for the timing, magnitude, and sustainability of northern water resources under continued climate warming.

How to cite: Baraer, M., Charonnat, B., Valence, É., Tjoelker, A., McKenzie, J., Masse-Dufresne, J., Dimech, A., and Mark, B.: Transient hydrosystems in deglaciating subarctic catchments: insights from a decade of research in the St. Elias Mountain Green Belt, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15188, https://doi.org/10.5194/egusphere-egu26-15188, 2026.

EGU26-16281 | ECS | Posters on site | GM9.3

Surface flow and internal structure of glacier-moraine complex (GMC) in northern Tien Shan 

Taiki Arai, Chiyuki Narama, Sagynbek Satarov, Daiyrov Mirlan, and Koyo Mizuno

In the northern Tien Shan, numerous glacier–moraine complexes (GMCs) composed of debris and ice have developed in front of glacier termini in this semi-arid region, but the conditions under which internal ice is maintained remain unclear. In this study, we investigated GMCs in front of the Adygine Glacier, located in the Kyrgyz Range of the northern Tien Shan, to clarify the relationship between internal structure and surface morphology. Electrical resistivity tomography (ERT) surveys were conducted along 15 profiles with 48 electrodes at 5 m spacing in 2024 and 2025, and horizontal and vertical surface displacements were quantified using UAV-derived imagery.

The results showed that in the upper left bank, continuous flow from the glacier and connected subsurface ice were identified. In the middle left bank, although no surface flow was observed, continuous buried ice was present, accompanied by surface lowering. In the lower left bank, continuous buried ice connected to a tributary glacier was also detected. On the right bank, exposed bedrock was found in the upper part, where meltwater flowed over the surface without infiltration into debris. In the lower right bank, debris landforms were developed, but flow was weak and the frozen layer was discontinuous. These findings indicate that continuous ice supply from the glacier is crucial for maintaining subsurface ice within the GMC.

How to cite: Arai, T., Narama, C., Satarov, S., Mirlan, D., and Mizuno, K.: Surface flow and internal structure of glacier-moraine complex (GMC) in northern Tien Shan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16281, https://doi.org/10.5194/egusphere-egu26-16281, 2026.

EGU26-17259 | Orals | GM9.3

Changing Geo-Hydrological Regime Over the Changing Climate: Global North to Global South, A Case Study: Nelson River Delta, Canada, and Ganges Delta, India. 

Sohini Sinha Roy, Tamoghna Acharyya, Sarmistha Basu, Afshana Parven, and Anirban Mukhopadhyay

Deltas are globally considered as one of the most vital socio-ecological systems, however their geo-hydrological regimes are gradually destabilized by change in climatic patterns. Based on this scenario, the research delves into a comparative study of two contrasting deltas comprising of Nelson River Delta in Canada situated in Global North and the Ganga-Brahmaputra Delta spatially occupying India and Bangladesh situated in Global South. Both deltas are significant ecological systems; The Nelson delta is characterized by boreal-subarctic wetland ecosystems, fisheries and traditional livelihood, on the other hand, the Ganges Delta marks a region of high population density characterized by complex interplay of natural and anthropogenic activities, fisheries, intensive agriculture and mangrove ecosystems. Impact of climatic shifts are evident in both deltas. In the Nelson River basin, altered snowmelt regimes and river discharge, accelerated thawing of permafrost coupled with flow regulation are leading to alteration in sediment delivery, coastal stability and ice breaking processes. While, Ganga delta is subjected to intense monsoon variability, frequent cyclones, sea level rise are augmenting issues like salinity intrusion, sediment redistribution and subsidence. These fluctuations have reconfigured geo-hydrological hazards by escalating the frequency and magnitude of bank erosion, floods, wetland degradation and coastal retreat. The consequences extend surpassing the physical processes to extensive changes in life and livelihoods of the residents evident from shifts in fish productivity, agriculture, food security and infrastructure vulnerability. Ecosystem services comprising of storm protection, carbon storage, biodiversity support and freshwater provision are either being modified or lost in both the regions. The research emphasizes the requirement for climate-responsive, place-based planning that constitutes sediment management, nature-based solutions, hydrological restoration and community-centered governance. Establishing resilience in both Global North and South need inclusive, adaptive and ecosystem-oriented strategies that would address accelerating hydrological and climatic uncertainties.

How to cite: Sinha Roy, S., Acharyya, T., Basu, S., Parven, A., and Mukhopadhyay, A.: Changing Geo-Hydrological Regime Over the Changing Climate: Global North to Global South, A Case Study: Nelson River Delta, Canada, and Ganges Delta, India., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17259, https://doi.org/10.5194/egusphere-egu26-17259, 2026.

EGU26-18534 | ECS | Orals | GM9.3

 Climate-Driven Changes in Ice Phenology and Sediment Dynamics of the Masjok River, Northern Norway 

Jyoti Prakash Hati, Halina Kaczmarek, Rituparna Acharyya, Michał Habel, Paolo Porto, Marta Brzezińska, Berenger Koffi, Anirban Mukhopadhyay, and Monika Szymańska-Walkiewicz

The hydrological regimes in high-latitude river systems might be altered in future by climate change and its arctic amplification, leading to substantial changes in sediment concentrations and discharge. Ice cover and sediment dynamics in arctic and subarctic rivers also control nutrients and biogeochemical cycles, which have an impact on water quality and marine flora and fauna. Therefore, our primary objective is to detect the seasonal changes in the ice cover and sediment concentration in water in the subarctic estuary using remote sensing. The Masjok River is one of the major tributaries of the Tana River estuary, with a catchment area of ​​568.11 km², and was selected as the research area. Sediment transport in situ data were obtained during field missions in 2024 and 2025. River ice dynamics were observed using the Normalised Difference Snow Index (NDSI), and the seasonal variation of suspended sediment was observed using two indices, namely the Normalised Difference Suspended Sediment Index (NDSSI) and the Normalised Difference Turbidity Index (NDTI). The Google Earth Engine (GEE) platform was used for creating the indices using Sentinel-2 MSI datasets. The results of this study indicate that suspended sediment concentrations and turbidity are high during the spring ice breakup season and lower in winter. Ice melting in the river and surrounding valleys generates very high spring discharge, which accelerates erosion and transports large sediment loads from the Masjok River to the Tana River. The first day of ice-free conditions in the Masjok River and surrounding areas occurs earlier. At the same time, the long-term discharge data suggest there was no drop in total and maximum discharge in the last 30 years. The experimental framework offers a comprehensive analysis of the interactions between ice, sediment, and discharge in the context of climate change. The findings of this research will advance the modelling of Arctic hydrology, which has significant ramifications for the management of water resources, ecological monitoring, and sediment transport in the Arctic.

Keywords: Masjok River, suspended sediment, turbidity, river ice-cover, Sentinel-2.

This research is financed by grant RID/SP/0048/2025/01, Ministry of Science and Higher Education, Title: Influence of environmental drivers on the variability of fine sediment transport in a subarctic river – case study of the Tana River, PI: Marta Brzezińska, Kazimierz Wielki University

How to cite: Hati, J. P., Kaczmarek, H., Acharyya, R., Habel, M., Porto, P., Brzezińska, M., Koffi, B., Mukhopadhyay, A., and Szymańska-Walkiewicz, M.:  Climate-Driven Changes in Ice Phenology and Sediment Dynamics of the Masjok River, Northern Norway, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18534, https://doi.org/10.5194/egusphere-egu26-18534, 2026.

EGU26-19350 | ECS | Posters on site | GM9.3

Reconstructing glacier-controlled sediment connectivity through time: Late Quaternary landscape evolution in the southeastern Alps 

Camilla Vidi, Giovanni Monegato, Sandro Rossato, Marco Cavalli, Stefano Crema, and Alessandro Fontana

Sediment (dis)connectivity is a fundamental concept for the understanding of landscape evolution and sediment fluxes, yet its long-term variability across contrasting climatic and glacial conditions remains poorly constrained. In particular, glaciers are commonly treated as purely erosional agents, while their role in structuring sediment pathways and storage through time is still underexplored.

In this study, we investigate the evolution of sediment connectivity during key phases of Late Quaternary landscape development, from the pre-Last Glacial Maximum (>30 ka), the Late Late Glacial (~14.7–11.7 ka), to the present. The Terragnolo Valley, an Alpine catchment in the southeastern European Alps, provides an ideal natural laboratory, having been repeatedly shaped by glaciations involving both a local glaciares and the Adige trunk glacier (>1000 m thick), resulting in an exceptional abundance of glacial and proglacial deposits.

We adopt a methodological framework that explicitly considers glaciers and associated sedimentary bodies as dynamic controls on sediment (dis)connectivity within a watershed. High-resolution palaeotopographies (2 m DTMs) are reconstructed for each target time slice by integrating detailed geomorphological mapping, stratigraphic constraints, and terrain modelling techniques. Sediment connectivity is quantified using the Index of Connectivity (IC; Borselli et al., 2008; Cavalli et al., 2013), accounting for time-dependent forcing factors such as ice extent and evolving topographic configuration.

The IC-based analysis is complemented by field-based geomorphological observations, with particular attention to the identification of buffers and barriers following the conceptual framework of Fryirs et al. (2007). With this approach, we aim to reconstruct past sediment pathways and to explore how glacial dynamics promoted sediment storage, fragmentation of connectivity, or, conversely, efficient sediment transfer. Connectivity under modern conditions is computed using the SedInConnect software (Crema and Cavalli, 2018while specific topographic reconstruction enable its application to palaeolandscapes.

Our results aim to elucidate how glacier-driven landscape reorganization controlled sediment distribution and led to the development of disproportionate sediment accumulations in specific sectors of the catchment. By reconstructing sediment connectivity through multiple glacial–interglacial transitions, this study provides new insights into the long-term controls on sediment fluxes in Alpine environments and offers a framework for contextualizing present-day sediment dynamics within their Quaternary context.

How to cite: Vidi, C., Monegato, G., Rossato, S., Cavalli, M., Crema, S., and Fontana, A.: Reconstructing glacier-controlled sediment connectivity through time: Late Quaternary landscape evolution in the southeastern Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19350, https://doi.org/10.5194/egusphere-egu26-19350, 2026.

Glacier forelands are hotspots of accelerated environmental change in high mountain environments. As landscapes transition from glacial to non-glacial conditions, they undergo pronounced geomorphic and ecological disequilibrium driven by paraglacial adjustment and primary succession. These coupled dynamics control sediment redistribution, disturbance regimes, and emerging ecosystem functions. Yet, despite extensive local-scale research, there is still a lack of integrated, comparative datasets that quantify foreland development trajectories across sites and environmental gradients.

We build on the Austrian Glacier Inventory outline series (GI LIA ~1850; GI1 1969; GI2 1998; GI3 2006; GI4 2015; GI5 2023, forthcoming) to reconstruct retreat-derived surface-age domains across 582 Austrian glacier forelands exposed since the Little Ice Age maximum. Surface-age domains are derived from successive inventory differences, providing discrete deglaciation-stage units for chronosequence-based comparisons across contrasting geomorphic and climatic settings.

For the remote sensing component, we use Google Earth Engine–derived Landsat NDVI time series (1985-2025) to quantify vegetation development across glacier forelands, with Sentinel-2 integrated for recent high-resolution trajectories. Annual NDVI layers are generated as cloud-masked August 90th-percentile composites to represent near-peak seasonal vegetation conditions while minimising snow and cloud contamination. We extract annual mean NDVI and fractional vegetation cover (NDVI > 0.2) for each surface-age domain.

To link vegetation stabilisation with geomorphic forcing, we derive DEM-based predictors (e.g., slope, curvature, roughness, topographic wetness, and flow concentration) to delineate surface-process domains and terrain-based disturbance potential. This enables evaluation of how terrain setting and hydrologic controls modulate vegetation establishment, persistence, and disturbance-driven setbacks.

First results show pronounced heterogeneity in greening and stabilisation signals among Austrian glacier forelands. A pixel-based comparison of multi-year NDVI medians (2020-2024 minus 1985-1989) yields ΔNDVI values from −0.37 to +0.84. Classifying ΔNDVI into four greening/stability classes indicates that no–minor change dominates at the foreland scale (median ~70%), while moderate greening is widespread (median ~21%) and negative/unstable trends typically remain limited (median ~5%) but locally concentrate into persistent disturbance corridors, particularly in high-disturbance process domains.

Field validation in summer 2026 will combine stratified vegetation and geomorphic plot surveys with UAV-based orthomosaics and surface models across 15 representative forelands. This effort will be complemented by existing high-resolution datasets from Austria’s two largest forelands (Pasterze and Gepatschferner), supporting calibration of vegetation fractions and attribution of stabilisation trajectories to process-domain characteristics and surface mobility indicators. Together, these components form an integrated national baseline for cross-site analysis and long-term monitoring of glacier-driven surface-process and ecosystem trajectories. This contribution provides the basis for a public Austrian glacier-foreland vegetation change inventory and invites collaboration on validation, process interpretation, and cross-regional comparisons.

How to cite: Haselberger, S.: Towards an Austrian Glacier Foreland Inventory: Multi-decadal Greening Trajectories Linked to Terrain-based Disturbance Potential, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20049, https://doi.org/10.5194/egusphere-egu26-20049, 2026.

Abstract

Arctic river delta systems are complex settings in which hydrological connectivity among river systems, distributaries, and lakes governs sediment transport, productivity, and resilience. Given the current state of Arctic climate intensification and the subsequent permafrost thaw, understanding these relationships has become increasingly crucial; however, progress has been hindered by the polar regions' inaccessibility and large spatial extent. In this paper, a satellite-based method for identifying connectivity between lakes and rivers using the Normalized Difference Suspended Sediment Index (NDSSI) derived from Sentinel-2 imagery is presented for the Mackenzie Delta region in north-western Canada. Regarding this investigation, multispectral optical imagery acquired during snow-free periods in 2023 - 2025 was used to examine spatial and seasonal changes in suspended sediment concentration and the influence of snow and ice using the Normalized Difference Snow Index (NDSI). NDSSI values were compared with in-situ turbidity measurements from August 2023 and September 2025, indicating a strong and statistically significant relationship (r = 0.79, p < 0.001). Based on sediment signal intensity and the relationship between lakes and distributary channels, 34,448 lakes in the south-eastern delta were classified as permanently connected, seasonally connected, or hydrologically isolated. The findings indicate that sediment-optical signatures reliably identify active hydrological connections, particularly during the flood recession period when river sediment input is at its peak. The results demonstrate that NDSSI can detect concealed hydrological pathways in complex Arctic delta landscapes and provide a scalable metric for monitoring sediment dynamics and connectivity as climate and permafrost conditions evolve.

Keywords: Mackenzie Delta; hydrological connectivity; lake–river exchange; suspended sediment dynamics

This research is being conducted with the permission of the Government of Canada – North West Territories (NWT) – research licence number 17694 which was issued under application number 6131 and financed by grant National Research Centre in Poland no. 2024/53/B/ST10/03483: Arctic deltas as sponges: How do river deltaic plains now filter and trap sediment and carbon?

How to cite: Acharyya, R. and Habel, M.: Monitoring Lake–River Pathways: Remote sensing-based Detection of Sediment-Driven Connectivity across the Arctic Mackenzie Delta, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20215, https://doi.org/10.5194/egusphere-egu26-20215, 2026.

The Greenland Ice Sheet (GrIS) is a hotspot for sediment transport, where glaciers and their meltwaters deliver sediment and associated nutrients to proglacial outwash plains and the ocean. This outflux supports proglacial and marine ecosystems, where enhanced primary production can contribute to atmospheric CO2 drawdown and negative carbon feedback loops. As field measurements of sediment export from the GrIS are limited both spatially and temporally, we use Google Earth Engine to extract suspended sediment concentrations from Sentinel-2 near infrared reflectance measurements of meltwater flows exiting land terminating glacier systems in Greenland (ground truthed by field data from Watson River, Kangerlussuaq), where sediment export analysis is facilitated by meltwater estimates from the Regional Atmospheric Climate Model (RACMO). Over the summer meltwater seasons of 2016 – 2024 we estimate a combined mean annual sediment flux of ~0.44 Gt yr-1, where we note that export has increased at an average rate of ~0.001 Gtyr-1 over the study period. Land terminating glaciers of the GrIS exported the greatest suspended sediment flux of 0.51 Gtyr-1 in 2022 and the lowest export of 0.24 Gtyr-1 in 2018. Regionally, southwest Greenland provides the greatest suspended sediment export per area, accounting for ~41% of total export over the study period. Our analysis provides the first estimate of proglacial sediment export from all land-terminating glacier systems in Greenland using Sentinel-2 imagery, allowing us to examine drivers of change and establish a baseline for assessing future changes in sediment delivery, as a result of climate warming. These changes will alter land systems in front of glaciers and impact sediment-derived nutrient delivery/ ecosystem response, with resultant implications for CO2 drawdown.

How to cite: Bartlett, H., Winter, K., Ross, N., Lea, J., and Woodward, J.: Suspended sediment export from land-terminating glaciers of the Greenland Ice Sheet (2016 – 2024), calculated from Sentinel-2 near infrared reflectance measurements, processed in Google Earth Engine, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21030, https://doi.org/10.5194/egusphere-egu26-21030, 2026.

EGU26-21378 | ECS | Posters on site | GM9.3

Role of deltaic lakes as hydraulic filters: sediment sorting in the Arctic river delta under changing flow regimes 

Marta Brzezińska, Michał Habel, Damian Ciepłowski, Monika Szlapa, Dawid Szatten, and Anirban Mukhopadhyay

Ongoing climate change accelerates the degradation of permafrost, leading to an increased supply of meltwater and an intensified delivery of mineral sediments and organic matter to riverine and deltaic systems. Consequently, understanding the processes of hydraulic sorting and particle retention within deltaic environments, which determine the sediment budget and the “filtration efficiency” of these systems at the scale of the entire Arctic, becomes of critical importance.
The aim of this study is to identify the influence of hydraulic sorting mechanisms on changes in the size and concentration of suspended sediment particles during the passage of meltwater through the deltaic system of a large Arctic river. The study area is the lake-rich central part of the Mackenzie Delta (Canada, Northwest Territories). The experiment was conducted from the onset of ice-cover degradation until the end of the summer season, tracing the pathway of water transferred from the East Channel to the Middle Channel over a distance of approximately 12 km through three lakes permanently connected to the distributary channel network. Five monitoring stations for suspended sediment concentration (SSC) were installed, and measurements were carried out on eleven occasions between 24 May and 10 September 2025. In total, 120 suspended sediment samples were analysed.
The material was subjected to laboratory analyses of SSC and grain-size distribution using laser diffraction. The results show that, during the initial phase of observations, suspended sediments in the cold waters of the Mackenzie Delta (0.5–1.7°C) were characterized by SSC values ranging from 68 to 218 mg·l⁻¹ and by a bimodal grain-size distribution. In contrast, samples collected during the falling limb of the freshet (June–July) and during low-flow conditions (August–September) exhibited much lower SSC values, ranging from 10 to 68 mg·l⁻¹. Grain-size analyses indicate that, with increasing residence time of water in the lakes, a clear hydraulic sorting of particles according to their size occurs. This process results in the selective retention of coarser particles and aggregates within the lake zones, while finer silt–clay fractions continue to be transported towards the lower parts of the delta.
The dominant modal peak corresponds to the clay–silt fraction, typical of wash load, whereas a second peak in the range of 200–1000 µm, representing coarse and very coarse sand, appears only episodically during periods of increased discharge and enhanced turbulence. The fractional composition of suspended sediments at the end of May 2025 indicates a dominance of silt (70–85%), with clay contents of 5–10% and sand contents of 10–20%, of which the very coarse fraction (>250 µm) occurred only sporadically (<5%). This material can be classified as fine silt-dominated wash load with low settling velocities.
The obtained results confirm the key role of channel-adjacent lakes as natural hydraulic filters in Arctic deltas and demonstrate that hydraulic sorting of particle sizes and variability in settling dynamics are directly controlled by the hydrological regime of the spring freshet, the intensity of flow turbulence, and the cyclic processes of flocculation and destruction of sediment aggregates.

This research is financed by grant National Research Centre in Poland no. 2024/53/B/ST10/03483

How to cite: Brzezińska, M., Habel, M., Ciepłowski, D., Szlapa, M., Szatten, D., and Mukhopadhyay, A.: Role of deltaic lakes as hydraulic filters: sediment sorting in the Arctic river delta under changing flow regimes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21378, https://doi.org/10.5194/egusphere-egu26-21378, 2026.

EGU26-21891 | ECS | Orals | GM9.3

Modeling the Alps across large spatial and temporal scales using theInstructed Glacier Model (IGM) 

Brandon D. Finley, Guillaume Jouvet, Maxime Bernard, Tancrede P.M. Leger, Guillaume Cordonnier, and Frederic Herman

The European Alps and its unique features were largely formed from additive processes like
sediment deposition and subtractive processes such as glacial erosion. Spanning millions of
years, these processes that helped shape the Alps are not fully understood due to their complexity
and tenancy to be coupled with each other. Existing landscape evolution models that include
these processes are limited in their computational power - often only allowing a coarser spatial
resolution. A high spatial resolution, and by extension maintaining higher-order physics fidelity,
is also imperative in accurately reconstructing the Alps. We aim to address this limitation by
using the community-led Instructed Glacier Model (IGM) that leverages Graphical Processing
Units (GPUs) and scientific machine learning (SciML) to accelerate computation. Here, we adapt
IGM to be a landscape evolution model (LEM) by including relevant mechanisms for landscape
evolution such as glacial abrasion, quarrying, fluvial erosion, isostatic rebound, and hill-slope
processes.

To demonstrate its capacity, we first benchmark its results against traditional landscape evo-
lution models (i.e. iSOSIA), validating that, though IGM is a physics-informed machine learning
model, it remains a process-based LEM. We furthermore aim to show its efficiency at modeling
across a wide range of scales such as multiple alpine catchments as well as longer temporal
periods such as during the Quaternary. As such, we hope our modeling approach can be used
for various applications such as exploring how glaciers are linked to these underlying processes,
inverse problems to achieve better model-data agreements, and ensembles across long temporal
or spatial scales.

How to cite: Finley, B. D., Jouvet, G., Bernard, M., Leger, T. P. M., Cordonnier, G., and Herman, F.: Modeling the Alps across large spatial and temporal scales using theInstructed Glacier Model (IGM), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21891, https://doi.org/10.5194/egusphere-egu26-21891, 2026.

CR3 – Sea, Lake and River Ice

EGU26-208 * | Orals | CR3.1 | Highlight

Sea-ice ridges - an understudied yet key component of the Arctic sea-ice system 

Mats A. Granskog and the HAVOC (MOSAiC) team

Sea-ice ridges (or more precisely, deformed ice) constitute a large fraction of the Arctic ice pack, however, estimates range broadly from 30 to 70%. Yet, we know disproportionally little about their role in the Arctic sea-ice system, a system that is in rapid change. In situ studies of ridges are logistically challenging, and as a result, most research has focused on level sea ice, despite the significant proportion of sea ice residing in ridges.

Ridges evolve over time and provide an environment for ice growth very different than the typical level ice. Observations during the year-long MOSAiC drift expedition revealed several processes that could contribute to ice growth, even in summer, when most of the ice pack is melting. Indirectly ridges also affect, for example, melt pond formation, and also under-ice spreading of meltwater (under-ice ponds), that  in turn affect the melt rates of level ice. However, these indirect effects of ridges have virtually never been quantified.

Rare observations from the MOSAiC expedition explored the unique habitats within sea-ice ridges, including surfaces of ice blocks in association with water-filled voids, showed distinct differences in biological properties compared to level ice bottom and pelagic biota. These ridge-specific habitats had unique protist and bacterial assemblages contributing to the high diversity and richness found in Arctic sea ice. In summer, ridges can be hotspots of protist biomass and can contain the majority (up to 80%) of sea ice algal biomass - an element not yet considered in Arctic assessments of sea-ice biomass.

We argue that sea-ice ridges should be included in assessments of Arctic Ocean biodiversity and biogeochemistry to fully understand the Arctic sea-ice ecosystem and its response to ongoing changes. Future efforts should not only investigate the complex physical and biological processes within sea-ice ridges but also integrate these processes into models. Only then can we predict how the changes in the Arctic icescape will affect atmosphere-ice-ocean-ecosystem interactions and how the ongoing changes of the ice pack will affect ridging in the future.

 

 

How to cite: Granskog, M. A. and the HAVOC (MOSAiC) team: Sea-ice ridges - an understudied yet key component of the Arctic sea-ice system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-208, https://doi.org/10.5194/egusphere-egu26-208, 2026.

Melt ponds formed during summer play a crucial role in the evolution of Arctic sea ice. Observations show that the salinity in melt ponds ranges from 1 to 29 PSU, and saline ponds have different thermal properties from freshwater ponds. During the melt season, ponds with different salinities can exhibit distinct flow regimes and heat-transport efficiencies under the same radiative forcing, which can affect the relative fractions of absorbed heat that is emitted back to the atmosphere versus down into the ice. These feedbacks thus impact the evolution of pond depth. In the freezing season, the brine solution within a pond forms a porous mushy layer as it solidifies. If gravity drainage is triggered, the resulting plumes may induce complex circulation within the remnant unfrozen liquid beneath the ice lid and modify salinity transport within the underlying ice layer. These effects have not yet been fully quantified in existing models, despite their potential impact on the coupled pond–ice system.

We develop a one-dimensional pond-ice model based on an enthalpy method and a brine drainage model to explore how initial pond salinity influences the system over a melting–freezing cycle. We constrain the parameterised fluxes in the one-dimensional model using insight from a suite of two-dimensional high-resolution simulations, including double-diffusive convection and mushy-layer dynamics. Our two-dimensional simulations of double-diffusive convection during the melting stage show that salinity regulates the internal flow regime by controlling stratification, thus inhibiting turbulent convection at relatively high salinities. During the refreezing stage, two-dimensional simulations using the enthalpy method show that gravity drainage can occur across a wide salinity range, initiating turbulence even in the absence of external heat sources. This turbulence leads to highly efficient vertical salt transport. By varying the initial salinity in the one-dimensional model, we find that salinity can consequently influence both the maximum pond depth and the timescale of pond refreezing.

How to cite: Zhang, Y. and Wells, A.: A One-Dimensional Enthalpy Model for Melt and Refreezing of Saline Arctic Melt Ponds Constrained by Two-Dimensional Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1093, https://doi.org/10.5194/egusphere-egu26-1093, 2026.

EGU26-1462 | Posters on site | CR3.1

High resolution monitoring of sea ice properties with Distributed Acoustic Sensing 

Ludovic Moreau, Sebastien Kuchly, Antonin Eddi, Stéphane Perrard, and Dany Dumont

To understand the response of sea ice to geophysical forcing, collecting field data remains essential. However, in situ monitoring of sea ice physical properties is challenging due to the complex logistics of the polar environment. Remote sensing methods such as Synthetic Aperture Radar (SAR) address some of these logistical constraints, but typically provide spatial information at regional scales and with temporal resolutions on the order of several days. While this is sufficient for large-scale monitoring, current sea ice models still struggle to accurately reproduce its decline, partly because small-scale processes are not adequately captured. Consequently, the next generation of models will require finer resolutions to describe local-scale ice–ocean interactions, especially in the context of the expanding Marginal Ice Zone (MIZ). This need is closely linked to our ability to observe small-scale sea ice properties so that breakup mechanisms associated with swell forcing can be better understood.

We introduce a methodology based on Distributed Acoustic Sensing (DAS) to recover small-scale variations in ice thickness and Young’s modulus. We test this approach on a dataset recorded in February 2025 on fast ice in the St. Lawrence Estuary (Canada). We demonstrate that sea ice properties can be estimated from both active and passive acquisitions on distances of the order of the km, with a spatial resolution of ~20 m.   

How to cite: Moreau, L., Kuchly, S., Eddi, A., Perrard, S., and Dumont, D.: High resolution monitoring of sea ice properties with Distributed Acoustic Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1462, https://doi.org/10.5194/egusphere-egu26-1462, 2026.

EGU26-2520 | Posters on site | CR3.1

Effects on the transition zone of retreating seasonal sea ice in the Baltic Sea 

Ülo Suursaar, Martin Mäll, Katre Luik, and Hannes Tõnisson

According to Copernicus data, the last three years (2023–2025) have been the hottest on record globally. In Northern Europe, however, the pace of warming has even exceeded the global average. This case study focuses mainly on the Estonian coastal area of the Baltic Sea, where air temperatures at coastal stations have risen by about 2.5°C between 1950 and 2025. As a result, the annual maximum Baltic Sea ice extent has declined (according to the endpoints of a linear trend) from 212 to 140 thousand km² (34%) over the centennial period between 1924/25 and 2024/25, and ice-cover duration in the Estonian coastal sea has decreased, depending on the station, by roughly 30–60% since 1950. This decline has likely contributed to the intensification of coastal erosion observed along several Estonian coastal stretches and more broadly along the southeastern Baltic Sea.

The study reviews shifts in ice-related processes with coastal geomorphic consequences, including changes in wave conditions due to longer ice-free seasons, reduced effective fetch, and shorter periods of frozen coastal sediments. Two less-studied effects are examined in detail: (1) using the ERA5-forced WRF–FVCOM modelling suite to quantify how the absence of ice affects sea-level patterns in the Gulf of Riga and the suppression of sea-level maxima during winter storms; and (2) analysing the occurrence and impact of winter (“warm”) upwelling on ice dynamics using ADCP measurements, meteorological–oceanographic observations, ice charts, and SST imagery.

The results show that reduced ice cover can help explain the higher storm surges observed in the Baltic Sea. In recent, more ice-free decades, winter storms have more freely produced surges, whereas before the 1980s they were often suppressed by sea ice. The combination of declining ice cover and the increasing probability of undamped storm surges likely contributes to steeper sea-level maxima and higher upper-quantile sea-level trends in long-term records. Secondly, although coastal upwelling in the Baltic Sea is usually considered a summertime process, similar forcing in winter can bring slightly warmer subsurface water (2–4°C) to the surface, contrasting with pre-freezingly cooled (0–1°C) surface water. The process is quite frequent along the straight North Estonian coast of the Gulf of Finland, when during sustained easterly winds this upwelled water creates a stark contrast with cold (–10…–20°C) weather conditions in the area. The phenomenon often delays coastal ice formation relative to the Finnish side and may help explain an anomaly in regional ice-pattern statistics in the mouth section of the Gulf of Finland.

Finally, as the transition zone between ice-free and seasonally frozen seas shifts northward under climate warming, the regions affected by these processes will also migrate. Winter upwelling has little effect in seas that are either fully ice-free or that freeze over rapidly. It is likely that about a century ago these processes were more pronounced south of Estonia (e.g., along the Latvian and Lithuanian coasts), and in the future they may shift farther north, such as into the Bothnian Sea. 

How to cite: Suursaar, Ü., Mäll, M., Luik, K., and Tõnisson, H.: Effects on the transition zone of retreating seasonal sea ice in the Baltic Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2520, https://doi.org/10.5194/egusphere-egu26-2520, 2026.

EGU26-4061 | ECS | Posters on site | CR3.1

Exploring the role of ocean preconditioning as a driver of Antarctic sea ice loss events 

Adam Bateson, Daniel Feltham, Birgit Rogalla, Tarkan Bilge, Kaitlin Naughten, Paul Holland, Caroline Holmes, and David Schröder

Antarctic sea ice expanded during much of the late 20th and early 21st century, in contrast to the rapid loss of sea ice observed in the Arctic over the same period. However, since the mid-2010s, Antarctic sea ice has produced a series of record minima, with 2022 – 2025 collectively producing the lowest four extents on record. Climate models with adequate global warming have struggled to reproduce the general increase in sea ice coverage prior to 2016 and only very rarely simulate losses of the magnitude seen thereafter, raising concerns about their capability in simulating realistic variability in Antarctic sea ice state. Moreover, climate models have significant Southern Ocean biases, in particular an overestimation of Southern Ocean convection, which is a related source of low confidence in sea ice variability. Understanding the relationship between sea ice variability and the Southern Ocean state is particularly important because several recent studies have suggested that warming in the subsurface ocean is a significant driver of the repeated sea ice lows seen in the Antarctic since 2016.

In this study, we identify a series of substantial sea ice loss events within model output from simulations produced using a regional Southern Ocean circumpolar configuration of NEMO-SI3. We also characterise the modelled ocean salinity and temperature profiles leading up to each ice loss event. We then run a series of sensitivity studies where we either directly modify the ocean state or change parameters that impact the subsurface ocean. We will present results exploring how the magnitude of ice loss events is impacted by these changes in ocean state and discuss the implications of these results for the role of the ocean as a driver of Antarctic sea ice change and variability.

How to cite: Bateson, A., Feltham, D., Rogalla, B., Bilge, T., Naughten, K., Holland, P., Holmes, C., and Schröder, D.: Exploring the role of ocean preconditioning as a driver of Antarctic sea ice loss events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4061, https://doi.org/10.5194/egusphere-egu26-4061, 2026.

EGU26-4698 | Posters on site | CR3.1

Injection-Latitude Dependence of Arctic Sea Ice Recovery in Stratospheric Aerosol Injection Simulations 

Hyerim Kim, Hyemi Kim, Daniele Visioni, and Ewa Bednarz

Under multiple anthropogenic warming scenarios in CMIP6, Arctic sea ice is projected to undergo a rapid seasonal decline by the mid-21st century. Stratospheric Aerosol Injection (SAI) has been proposed as a potential intervention to mitigate Arctic warming, yet the sensitivity of Arctic sea-ice recovery to aerosol injection latitude, including its magnitude and governing processes, remains insufficiently quantified. Here, we investigate how SAI injection latitude influences Arctic sea ice recovery using simulations with CESM2-WACCM6, in which sulfate aerosols are injected at latitudes ranging from 45°S to 45°N under fixed injection rates.

Our results show that Arctic sea ice recovery exhibits a strong dependence on injection latitude, with injections closer to the North Pole producing a more rapid and robust recovery in both sea-ice extent and volume. This response is associated with coordinated changes in clear-sky and cloud radiative fluxes, as well as enhanced surface albedo, which together favor a surface energy balance conducive to ice growth. Notably, we find that Arctic sea ice recovery does not scale linearly with global mean surface temperature under SAI, highlighting the importance of injection latitude in shaping regional cryospheric responses.

How to cite: Kim, H., Kim, H., Visioni, D., and Bednarz, E.: Injection-Latitude Dependence of Arctic Sea Ice Recovery in Stratospheric Aerosol Injection Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4698, https://doi.org/10.5194/egusphere-egu26-4698, 2026.

EGU26-5123 | ECS | Posters on site | CR3.1

A regime change in Arctic sea ice growth 

Benjamin Mellor, Michel Tsamados, and Harry Heorton

The decline in Arctic sea ice thickness (SIT) is a key indicator response of the cryosphere to anthropogenic climate change. While the drivers of this decline are debated, they involve a competition between the ice-albedo positive feedback that enhances ocean heat content and the thin-ice negative feedback enhancing ice speed and alters dynamic-thermodynamic interactions. To date, pan-Arctic assessments of the dynamic and thermodynamic responses have been limited to the CryoSat-2 era (2010–Present Day).

Here we apply recently developed thickness products to produce novel 30-year records of Arctic sea ice volume (SIV) budget, resolving dynamic and thermodynamic terms. Our residual growth is validated on IMB buoy data and has a slight positive bias of +0.14 m-1 and a strong seasonal cycle. We identify a step change increase of 1,300 km-3 in thermodynamic growth, coincident with the pause in volume decline of the winter of 2007/08, representing a regime change in system behaviour where 76\% of seasonal growth is explained by the mean thickness of the surviving sea ice (p<0.001). Furthermore, enhancement in growth is regionalised and strongly correlates with sea ice drift modes. Specifically, we find that cyclonic atmospheric circulation modes associated with a negative Arctic Oscillation promote a dynamically coupled thin-ice feedback by enhancing thermodynamic growth through divergence and advection of SIV. This effect is observed throughout the periphery seas and is variable on inter-annual and decadal timescales. Finally, we investigate the contribution of thickness, concentration and drift to budget term variance. Finding that 87% of volume flux variance is accounted for by SIT anomaly. We highlight the utility of volume budgeting for identifying unphysical spatio-temporal patterns in SIT datasets and provide a new long-term benchmark for constraining sea ice growth in climate model assessments.

How to cite: Mellor, B., Tsamados, M., and Heorton, H.: A regime change in Arctic sea ice growth, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5123, https://doi.org/10.5194/egusphere-egu26-5123, 2026.

EGU26-5368 | ECS | Posters on site | CR3.1

Effects of a landfast ice representation on Antarctic shelf water properties and ice shelf melt simulated by NEMO4-SI³ 

Noé Pirlet, Thierry Fichefet, Martin Vancoppenolle, Casimir de Lavergne, and Nicolas C Jourdain

The formation of dense water in the Southern Ocean plays a key role in the global ocean overturning circulation, affecting the distribution of heat, carbon, oxygen and nutrients across the World Ocean. However, its representation in large-scale ocean–sea ice models used in climate studies remains biased. These models often produce dense water in the wrong locations and for incorrect reasons. We hypothesize that this partly stems from a poor representation of coastal polynyas and their drivers, particularly landfast ice. In a recent study, we introduced a velocity-restoring method to represent Antarctic landfast ice in the NEMO4-SI³ ocean–sea ice model and demonstrated its essential role in shaping coastal polynyas and controlling sea ice production. Here, we investigate the impact of this landfast ice representation on Antarctic shelf water properties and ice shelf melt. When the landfast ice scheme is activated, continental shelf waters densify in some coastal polynya areas, as expected. However, freshening is also observed beneath extensive landfast ice tongues, influencing salinity in several downstream polynyas. At a circumpolar scale, landfast ice improves the realism of bottom shelf water salinity and temperature. Notably, changes in mixed layer depth modulate the exchanges between the continental shelves and the open ocean, resulting in enhanced ice shelf melt. Overall, we show that representing landfast ice impacts the simulated ocean stratification, and formation and transformation of key Antarctic water masses. Our results thus further highlight the need for a physically-based representation of Antarctic landfast ice in Earth system models.

How to cite: Pirlet, N., Fichefet, T., Vancoppenolle, M., de Lavergne, C., and Jourdain, N. C.: Effects of a landfast ice representation on Antarctic shelf water properties and ice shelf melt simulated by NEMO4-SI³, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5368, https://doi.org/10.5194/egusphere-egu26-5368, 2026.

EGU26-5640 | ECS | Posters on site | CR3.1

Detecting sea ice freeze-onset from Sentinel-1 synthetic aperture radar 

Mallik Mahmud and Benjamin Smith

The Canadian Arctic Archipelago is undergoing rapid climate-driven changes, including prolonged melt seasons and delayed freeze-up that accelerate the loss of thick multi-year ice. Existing freeze-onset datasets rely on localized in situ observations or coarse-resolution NASA passive microwave (PMW) products at km scale. However, in situ measurements lack systematic spatial coverage, while PMW data suffer from severe land contamination in the narrow channels and inlets of the Archipelago, limiting their reliability in this complex coastal environment. Detecting freeze-onset using high-resolution synthetic aperture radar (SAR) have historically been challenging due to sea ice motion that introduce uncertainty by disrupting pixel-level correspondence and backscatter continuity across image sequences. This study introduces a novel approach that integrates temporal backscatter slope analysis with environmental constraints, such as surface air temperature thresholds to overcome motion-related challenges. The method enables robust detection of freeze-onset events across both multi-year ice and open-water areas at 40 m pixel resolution, producing spatially comprehensive maps of freeze-up timing across the Canadian Arctic. Analysis during 2015–2025 will reveal fine-scale spatial and temporal variability in freeze-up patterns within the Last Ice Area. This work will deliver the first high-resolution freeze-up dataset for the Canadian Arctic, providing a scalable foundation for pan-Arctic freeze-onset estimation. 

How to cite: Mahmud, M. and Smith, B.: Detecting sea ice freeze-onset from Sentinel-1 synthetic aperture radar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5640, https://doi.org/10.5194/egusphere-egu26-5640, 2026.

EGU26-7024 | ECS | Orals | CR3.1

Formation of superimposed ice in Arctic : study from observations and modeling 

Louise Kilian, Jérôme Sirven, and Nathalie Sennéchael

The formation of superimposed ice on Arctic sea ice during the melt season is studied using in situ observations from ice mass balance instruments (SIMBA/IAOOS) and a one-dimensional thermodynamic model of snow and sea ice (LIM1D). Ice mass balance instruments measure vertical profiles of temperature and a proxy for thermal conductivity over a vertical extent of 5 m through the atmosphere, snow, ice and ocean at regular time intervals.

In this study, we analyse four time series from instruments deployed near the North Pole in April and drifting towards Svalbard, all of which clearly show periods of superimposed ice formation. The dataset covers three melt seasons (2013, 2015, and 2017). Air–snow, snow–ice, and ice–ocean interfaces are retrieved from the temperature and conductivity profiles with an accuracy of about 2 cm, but this uncertainty can become substantially larger during the melt period. Snowmelt periods are identified, and the subsequent formation of superimposed ice at the sea ice surface is estimated.

Numerical simulations with the LIM1D model are performed to complement the analysis of the observed time series. The sensitivity of the results to the atmospheric forcing is also analysed. Summer temperature profiles strongly depend on the longwave radiative flux. Simulations forced with ERA5 exhibit an earlier onset of snowmelt than observed, whereas experiments using ERA-Interim radiation lead to a substantially improved agreement with the observations. In contrast, variations in snow albedo and snow density have a limited impact during the pre-melt period.

The formation of superimposed ice is successfully reproduced by the LIM1D model. The role of precipitation and surface runoff in the days preceding superimposed ice formation, as well as the changes in sea ice suggested by the observations, are confirmed. Lastly, the deployment of the instruments modifies the surrounding environment and may influence local observations. This should be taken into account when interpreting ice mass balance measurements.

How to cite: Kilian, L., Sirven, J., and Sennéchael, N.: Formation of superimposed ice in Arctic : study from observations and modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7024, https://doi.org/10.5194/egusphere-egu26-7024, 2026.

EGU26-7684 | ECS | Posters on site | CR3.1

Comparing stress and deformation characteristics of sea ice using continuum and discrete element models 

Penelope Coulthard, Daniel Feltham, Adam Bateson, David Schroeder, and Ed Blockley

Most continuum models of sea ice follow the principles laid down by the Arctic Ice Dynamics Joint Experiment (AIDJEX), a US-Canadian initiative from the 1970s (McLaren, 1981). AIDJEX developed a model in which sea-ice floes break like a deformable plastic material at spatial scales of tens to hundreds of kilometres. This approach treats sea ice as a continuum, with the ice cover varying smoothly in space and time. Discrete element models (DEMs) model sea-ice floes as bonded groups of individual elements, explicitly capturing interactions with surrounding floes. Bond failure represents out-of-plane processes, such as ridging, or the formation of open water, such as leads.

We consider the results from simulating the dynamic and deformation properties of sea ice from a DEM and a continuum model using the same set of highly idealised scenarios. The results illustrate how the DEM can be used to provide an ensemble of possible outcomes around the mean behaviour provided by the continuum model, with the ensemble spread being linked to the spatial resolution being considered. The impacts of different stress confinement ratios are considered, illustrating a link between the DEM fracture patterns and fracture patterns that are observed in laboratory experiments on sea ice as well as in field observations.

Although the patterns of deformation from the DEM look more comparable to observed sea ice fracture patterns, the conclusions from this study support the use of continuum models for pack ice dynamics, especially at larger spatial scales.

How to cite: Coulthard, P., Feltham, D., Bateson, A., Schroeder, D., and Blockley, E.: Comparing stress and deformation characteristics of sea ice using continuum and discrete element models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7684, https://doi.org/10.5194/egusphere-egu26-7684, 2026.

EGU26-8600 | ECS | Posters on site | CR3.1

High-Resolution GNSS-Reflectometry Observations of Arctic Sea Ice from Taiwan’s Triton Satellite 

Hoa Duong, Hwa Chien, Ming-Yi Chen, Li-Ching Lin, and Wen-Hao Yeh

Taiwan’s Triton satellite carries a GNSS-Reflectometry (GNSS-R) payload designed to investigate bistatic L-band microwave scattering over the ocean and cryosphere. In this study, we present Arctic observations acquired during multiple overpasses from the late 2025 to early 2026, focusing on both the spatial coverage of specular points (SPs) and the physical interpretation of delay–Doppler map (DDM) signatures over sea-ice-covered regions.

Accumulated SP tracks over a three-months period demonstrate that Triton’s high-inclination orbit enables systematic sampling beyond 88°N, extending into the central Arctic Basin where conventional monostatic microwave sensors and existing GNSS-R missions, such as CYGNSS, do not provide coverage. In addition, Triton offers approximately four times higher resolution in both delay and Doppler dimensions compared to CYGNSS, enhancing sensitivity to subtle variations in surface scattering regimes.

Beyond spatial coverage, first-look analyses of high-resolution DDMs collocated with passive microwave sea ice concentration products reveal distinct scattering characteristics over marginal ice zone and partial ice cover conditions. Observed DDMs exhibit energy concentrated near the specular delay with pronounced elongation in the Doppler dimension, while remaining relatively confined in delay. This behavior is consistent with quasi-specular scattering from ice floes and reduced surface roughness.

The enhanced delay resolution further provides a framework to assess the potential contribution of subsurface or multi-layer reflections at L-band, which may become detectable under thicker or more consolidated ice conditions. These results indicate that high-resolution GNSS-R observations from Triton are sensitive not only to the presence of sea ice, but also to changes in scattering mechanisms related to ice structure and surface state. Ongoing work aims to systematically classify DDM observables across ice regimes and seasons, assessing the feasibility of GNSS-R as a complementary tool for Arctic sea ice characterization.

Figure. Spatial Cover over the Arctic region from 2025/10/02 to 2026/01/08 by TRITON satellite 

How to cite: Duong, H., Chien, H., Chen, M.-Y., Lin, L.-C., and Yeh, W.-H.: High-Resolution GNSS-Reflectometry Observations of Arctic Sea Ice from Taiwan’s Triton Satellite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8600, https://doi.org/10.5194/egusphere-egu26-8600, 2026.

EGU26-9496 | ECS | Posters on site | CR3.1

Anatomy of Arctic and Antarctic sea ice lows in an ocean–sea ice model 

Benjamin Richaud, François Massonnet, Thierry Fichefet, Dániel Topál, Antoine Barthélemy, and David Docquier

Sea ice has exhibited a number of record lows in both hemispheres over the past two decades. While the causes of individual
sea ice lows have already been investigated, no systematic comparison across events and hemispheres has been conducted
in a consistent framework yet. Here, the global standalone ocean–sea ice model NEMO4.2.2-SI3 at 1/4° resolution is used
to decompose the sea ice mass budget. We separate the relative contributions of ice melt/growth and thermodynamic/dynamic
processes, both from a climatological perspective and for selected individual years. The seasonal cycles of Arctic and Antarctic
ice mass fluxes show similarities, such as the prevalence of basal growth and melt in the mass budget. The long-term evolution
of the mass budget terms reveals an increased importance of basal melt in both hemispheres, at the expense of surface and
lateral melt. Regarding sea ice lows, the model indicates that the Arctic summer 2007 anomaly was chiefly caused by dynamic
factors, while the Arctic summer 2012 event was rather explained by thermodynamic factors. The Antarctic summer 2022 event
was driven by dynamic processes transporting ice towards sectors where more melt than usual occurred. The Antarctic winter
2023 event was characterized by a lack of basal growth. This study emphasises the dominance of processes at the ice-ocean
interface in driving the ice mass evolution at all time scales considered here, and highlights the potential of the ice mass budget
decomposition to disentangle oceanic and atmospheric contributions in the evolution of the ice state in a changing climate.

How to cite: Richaud, B., Massonnet, F., Fichefet, T., Topál, D., Barthélemy, A., and Docquier, D.: Anatomy of Arctic and Antarctic sea ice lows in an ocean–sea ice model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9496, https://doi.org/10.5194/egusphere-egu26-9496, 2026.

EGU26-9934 | ECS | Orals | CR3.1

Observing Arctic sea ice freeboard with high-resolution spaceborne grazing angle GNSS-Reflectometry 

Felix L. Müller, Robert Ricker, Edmond Hansen, Kevin Halsall, Matthieu Talpe, Jessica Cartwright, Denise Dettmering, Florian Seitz, Leonardo De Laurentiis, Alessandro Di Bella, and Jerome Bouffard

A consistent monitoring of the sea ice freeboard is crucial for observing changes in sea ice thickness and for improving sea ice forecasts. Mainly, area-wide freeboard heights are determined by using surface elevations from satellite altimetry missions like ESA's Earth Explorer Cryosat-2 and NASA's ICESat-2. A sudden failure or interruption of these altimeter missions would lead to significant data gaps in the central Arctic Ocean. Therefore, additional ways to determine sea level and freeboard based on remote sensing techniques are of great importance.

One of these additional techniques is grazing angle GNSS reflectometry (GA GNSS-R), which uses surface reflections from Global Navigation Satellite System (GNSS) signals to capture elevation information and characterize surface roughness. Here, we utilize reflections collected by up to 15 Spire Global nanosatellites. These nanosatellites record both the directly transmitted signal (line of sight) and the signal reflected from the surface , The signals are used to determine the delays in the measured phase compared to a modelled phase, from which the elevation of a reflecting surface is then derived. Accurate height estimation is feasible when the reflected signal remains phase‑coherent and retains right‑hand circular polarization at grazing incidence angles between approximately 5° and 30°. Under these conditions, smooth surfaces such as sea ice or calm water produce strong coherent reflections, whereas rougher ocean surfaces induce decorrelation and significantly weaker reflected signatures.

As part of the ESA Earthnet Data Assessment Project (EDAP+), a new approach is developed to derive sea ice freeboard from GA GNSS-R observations providing complementary information to satellite altimetry. One key advantage of Spire’ GA GNSS-R constellation is the high geographic density over the poles  and thus continuous coverage of high latitudes without a systematic polar observation gap, as is the case with altimetry missions. Geolocated surface reflections and elevation data provided by Spire Global are used to classify surfaces, to detect water openings within the sea-ice cover (e.g., leads), to retrieve local sea-surface elevations, and subsequently to derive along-track sectional freeboard heights from GA GNSS-R observations.

This study presents first monthly Arctic-wide freeboard maps for a complete winter season (2023/2024) and comparisons with upward-looking sonar measurements and CryoSat-2 freeboard products. Initial comparisons demonstrate that GNSS-R-derived freeboard provides valuable complementary information, particularly in regions with a dense data coverage, and achieves accuracy comparable to altimetry during autumn and early winter.

How to cite: Müller, F. L., Ricker, R., Hansen, E., Halsall, K., Talpe, M., Cartwright, J., Dettmering, D., Seitz, F., De Laurentiis, L., Di Bella, A., and Bouffard, J.: Observing Arctic sea ice freeboard with high-resolution spaceborne grazing angle GNSS-Reflectometry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9934, https://doi.org/10.5194/egusphere-egu26-9934, 2026.

EGU26-10675 | ECS | Posters on site | CR3.1

Recent improvements of the melt pond albedo parametrization in HIRHAM-NAOSIM 

Patrizia Schoch, Evelyn Jäkel, Wolfgang Dorn, and Manfred Wendisch

The spread of climate model results in terms of quantifying the sea ice surface albedo feedback is partly caused by the sensitivity of the simulated sea ice surface albedo to surface warming. The accurate representation of the Arctic sea ice and its evolution throughout the year, particularly in the melting period, is crucial to obtain reliable climate model projections.

The rapidly warming Arctic leads to changes in sea ice properties. Arctic sea ice is becoming younger, transitioning from rough multi-year ice to flatter first-year ice. This influences the distribution and occurrence of melt ponds, which increase surface heterogeneity during the melting season. As a result, the surface albedo is altered and modelling it becomes more complex. However, many models are not able to simulate ice properties, like surface roughness, which would be beneficial for simulating melt pond fractions. A new melt pond fraction parametrization for the coupled Arctic climate model HIRHAM-NAOSIM has been developed using satellite data. This new parametrization includes a retarded response to temperature changes with different change rates for thin and thick ice. By taking only surface temperature and ice thickness as input variables, this parametrization can be applied to many climate models. An offline analysis with satellite data shows a higher correlation between the new parametrization and satellite observations (R=0.71) compared to the old parametrization (R=0.62). The offline analysis, first model results, and a comparison of model results with MOSAIC and satellite observations will be presented. The effects of the new parametrization on the radiative energy balance will be discussed.

How to cite: Schoch, P., Jäkel, E., Dorn, W., and Wendisch, M.: Recent improvements of the melt pond albedo parametrization in HIRHAM-NAOSIM, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10675, https://doi.org/10.5194/egusphere-egu26-10675, 2026.

EGU26-11998 | ECS | Orals | CR3.1

Melt Onset of Arctic and Antarctic Sea Ice from Scatterometer Data 

Rui Xu, Qian Shi, Qinghua Yang, Jiping Liu, Jie Su, and Matti Leppäranta

The melt onset (MO) of sea ice plays a crucial role in the polar climate system and is detectable by satellite remote sensing. This study used scatterometer data to identify the melt onset dates of Arctic and Antarctic sea ice. The MO identified by this method primarily reflects early changes in the physical properties of the snow layer and is therefore usually earlier than the melt signals detected based on sea ice concentration data. Results show that the melt onset dates in both polar regions exhibit a clear latitudinal dependence. During the study period (2007-2022), no statistically significant long-term trends were found in the average MO for the entire Arctic or for any of its sub-regions. Instead, interannual variability dominates the temporal evolution of MO in the Arctic. Similarly, most Antarctic sub-regions show no significant trends, with the notable exception of the Ross Sea, where MO has advanced significantly. This study further analyzed the trends in the Arctic surface energy budget based on multiple time windows. The net surface energy flux shows a consistent and statistically significant increase only in the Bering Sea across all considered time windows, which supports the earlier MO observed in this region. Although the advance in MO in the Bering Sea does not reach statistical significance, its magnitude (-3 days/decade) is substantially larger than that in most other sub-regions. Following the pronounced decline in Arctic sea ice extent that began in 2007, the trend of advancing MO has not been statistically significant. The underlying mechanisms driving this recent change warrant further investigation.

How to cite: Xu, R., Shi, Q., Yang, Q., Liu, J., Su, J., and Leppäranta, M.: Melt Onset of Arctic and Antarctic Sea Ice from Scatterometer Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11998, https://doi.org/10.5194/egusphere-egu26-11998, 2026.

EGU26-12121 | ECS | Posters on site | CR3.1

Insights on the statistics of extreme Arctic sea ice conditions from the EC-Earth3 climate model 

Jerome Sauer, Giuseppe Zappa, Francesco Ragone, and François Massonnet

Various studies identified possible drivers of extreme Arctic sea ice reduction, such as observed in the summers of 2007 and 2012, including sea ice-ocean preconditioning, large-scale atmospheric circulation variability and synoptic-scale cyclones. However, a robust quantitative statistical analysis and a better understanding of the predictability of extreme sea ice lows are hindered by the small number of events that can be sampled in observations and numerical simulations. Recent studies tackled the problem of sampling climate extremes by using rare event algorithms, i.e., computational techniques developed in statistical physics to reduce the computational cost required to sample rare events in numerical simulations. Here we apply a rare event algorithm to ensemble simulations with the European community Earth-System-Model version 3 (EC-Earth3) to study extremes of intra seasonal pan-Arctic sea ice area reduction under present-day climate conditions. The rare event simulations produce sea ice area anomalies larger in magnitude than observed in 2012, and we compute statistically significant composite maps of dynamical quantities conditional on the occurrence of extremes with probabilities of less than 1%. We exploit the improved statistics of low sea ice states to study their drivers on synoptic to seasonal time scales, including a sea ice area and sea ice volume budget analysis to disentangle the roles of dynamic vs. thermodynamic forcing on the sea ice. On statistical average over the extremes, enhanced thermodynamic melting accounts for approximately 75% of enhanced sea ice area and volume loss and predominately occurs on the Pacific-North American side, while enhanced dynamic sea ice loss appears on the Eurasian side of the Arctic. Finally, we show that extreme sea ice lows are on average preceded by persistent cyclonic mean sea level pressure anomalies over the central to eastern Arctic during the spring-summer transition. These low-pressure systems promote sea ice loss thermodynamically due to enhanced moisture and heat flux convergence, cloudiness, surface downward longwave radiative fluxes and dynamically through the impact of anomalous winds on the transport of sea ice.

How to cite: Sauer, J., Zappa, G., Ragone, F., and Massonnet, F.: Insights on the statistics of extreme Arctic sea ice conditions from the EC-Earth3 climate model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12121, https://doi.org/10.5194/egusphere-egu26-12121, 2026.

EGU26-12450 | Posters on site | CR3.1

Melting, freezing and dynamics of Arctic sea ice: pack ice versus marginal ice zone  

Daniel Feltham, Adam Bateson, Rebecca Frew, and David Schroeder

As the summer Arctic sea ice extent has retreated, the marginal ice zone (MIZ) is becoming a larger fraction of the ice cover. The MIZ is defined as the region of the ice cover that is influenced by waves and for convenience here is defined as the region of the ice cover between sea ice concentrations (SIC) of 15 % to 80 %.

We use model simulations to analyse individual processes of ice volume gain and loss in the ice pack (SIC > 80 %) versus those in the MIZ. We use an atmosphere-forced, physics-rich, sea-ice-mixed layer model based on CICE, that includes a joint prognostic floe size and ice thickness distribution (FSTD) model including brittle fracture and form drag. Our model produces realistic simulations as compared with satellite observations of sea ice extent and PIOMAS (the Pan-Arctic Ice Ocean Modeling and Assimilation System) estimates of thickness.

We compare the ice cover and mass balance processes between the 1980s, 2010s and 2040s. The MIZ fraction of the July sea ice cover, when the MIZ is at its maximum extent, increases by a factor of 2 to 3, from 14 % (20 %) in the 1980s to 46 % (50 %) in the 2010s in NCEP (HadGEM2-ES) atmosphere-forced simulations. In a HadGEM2-ES forced projection, the July sea ice cover is almost entirely MIZ (93 %) in the 2040s.

Basal melting accounts for the largest proportion of melt in regions of pack ice and MIZ for all time periods. During the historical period, top melt is the next largest melt term in pack ice, but in the MIZ, top melt and lateral melt are comparable. This is due to a relative increase of lateral melting and a relative reduction of top melting by a factor of 2 in the MIZ compared to the pack ice. The volume fluxes due to dynamic processes decrease due to the reduction in ice volume in both the MIZ and pack ice.

For areas of sea ice that transition to being MIZ in summer, we find an earlier melt season: in the region that was pack ice in the 1980s and became MIZ in the 2010s, the peak in the total melt volume flux occurs 20(12) d earlier. This continues in the projection where melting in the region that becomes MIZ in the 2040s shifts 14 d earlier compared to the 2010s.

How to cite: Feltham, D., Bateson, A., Frew, R., and Schroeder, D.: Melting, freezing and dynamics of Arctic sea ice: pack ice versus marginal ice zone , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12450, https://doi.org/10.5194/egusphere-egu26-12450, 2026.

EGU26-12828 | ECS | Orals | CR3.1

Delayed yet abrupt Antarctic sea-ice loss from wind-induced upwelling of ocean subsurface heat 

Martina Zapponini, Dae-Won Kim, Wonsun Park, Thomas Rackow, Lettie Roach, Tido Semmler, and Thomas Jung

Over the last decade, Antarctic sea ice has experienced an abrupt and pronounced decline, the underlying causes of which remain incompletely understood. Using the eddy-permitting configuration of the coupled climate model AWI-CM3, we show that such an abrupt transition can result from wind-driven ocean–ice interactions. In the simulation, a sharp sea-ice collapse occurs in the late 2020s, after a prolonged period of relative stability. The decline begins in the Indian Ocean sector, where subsurface heat gradually accumulates beneath a persistently stratified surface layer. Episodic intensifications of the Southern Hemisphere westerlies, associated with positive phases of the Southern Annular Mode, can locally enhance wind-driven upwelling and weaken the upper-ocean buoyancy barrier. A pronounced event of this type, simulated in the late 2020s, is sufficiently strong to abruptly ventilate the accumulated Circumpolar Deep Water heat toward the surface triggering a rapid, but sustained, sea-ice retreat. In contrast, under the same forcing, the low-resolution configuration of the model exhibits a more surface-controlled warming regime with stronger upper-ocean stratification, limiting the ability of wind anomalies to induce a threshold-like transition and resulting in a more gradual, nearly monotonic sea-ice decline. These results highlight the key role of ocean stratification and wind–ocean coupling in enabling abrupt Antarctic sea-ice change.

How to cite: Zapponini, M., Kim, D.-W., Park, W., Rackow, T., Roach, L., Semmler, T., and Jung, T.: Delayed yet abrupt Antarctic sea-ice loss from wind-induced upwelling of ocean subsurface heat, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12828, https://doi.org/10.5194/egusphere-egu26-12828, 2026.

EGU26-13249 | ECS | Posters on site | CR3.1

A Weakened AMOC Could Cause Southern Ocean Temperature and Sea-Ice Change on Multidecadal Timescales 

Rachel Diamond, Louise Sime, David Schroeder, Laura Jackson, and Paul Holland

The Atlantic meridional overturning circulation (AMOC) could substantially weaken over the next century due to climate change. The Southern Ocean (SO) is a key control of global ocean circulation and climate. Here, we use the latest generation of climate models to assess the impacts of this potential AMOC weakening on the SO and Antarctic sea ice, on timescales of less than a century. Following AMOC weakening, ocean transports move heat southwards into the SO, causing SO surface warming and sea-ice loss. We also identify a new atmospheric connection, from the tropics to Antarctica: this connection enhances warming and sea-ice loss in one SO region, but causes cooling and sea-ice growth in another. This shows that substantial AMOC weakening could impact the SO on multidecadal timescales. However, these SO changes resulting from AMOC collapse are much smaller than the projected direct impacts of greenhouse-gas-induced warming.

How to cite: Diamond, R., Sime, L., Schroeder, D., Jackson, L., and Holland, P.: A Weakened AMOC Could Cause Southern Ocean Temperature and Sea-Ice Change on Multidecadal Timescales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13249, https://doi.org/10.5194/egusphere-egu26-13249, 2026.

EGU26-13285 | ECS | Orals | CR3.1

Reconstruction of a wave-induced ice break-up using unmanned aerial vehicles and stereo-DIC methods 

Sebastien Kuchly, Baptiste Auvity, Antonin Eddi, Dany Dumont, and Stéphane Perrard

Ocean waves can trigger sea ice fractures. This process plays an important role on the evolution of the floe size distributions in the marginal ice zone (MIZ). However, the fracture of sea ice by waves is still poorly constrainted by observations, as it is difficult to precisely forecast, it mostly occurs on short time (minutes) and spatial scales (meters), and are often happening during extreme weather conditions. In order to better understand the fracture of ice by waves, we built on the work of Dumas-Lefebvre et al. [1] and designed an experiment where waves are generated by an icebreaker nearby a continous ice sheet. This experiment was realized in the Saguenay Fjord, Québec, Canada, in February 2024, in the context of the Transforming Climate Action (TCA) program. The continuous 12-cm thick layer of ice that recently formed was fully characterised before the CCGS Amundsen generated wave by sailing at a speed up to 15.8 knots. Wave propagation and ice break-up were recorded by wave buoys placed on the ice surface and by three unmanned aerial vehicles (UAV) in stationary flights overseeing the ice from different angles.

Using digital image correlation (DIC), geometric projections and rectifications, we developed a method to recover the three components of the waves velocity field from UAV observations. The accuracy of the method has been tested using the buoy signals as a reference, showing a quantitative agreement with a relative error of about 5%. Thanks to this stereo-DIC method, we obtained the full wave velocity field over a grid of 106x75 meters with a spatial resolution of 0.8 pix/m and a sampling frequency of 30 Hz. This reconstruction method offers a precise, high spatio-temporal sampling needed for future characterization of sea ice fracture, or any other dynamics of textured surfaces.

References:

1. Dumas-Lefebvre, Elie and Dumont, Dany Aerial observations of sea ice breakup by ship waves TheCryosphere (2023)

How to cite: Kuchly, S., Auvity, B., Eddi, A., Dumont, D., and Perrard, S.: Reconstruction of a wave-induced ice break-up using unmanned aerial vehicles and stereo-DIC methods, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13285, https://doi.org/10.5194/egusphere-egu26-13285, 2026.

EGU26-15536 | Orals | CR3.1

Overshooting convective plumes and their role in winter Antarctic sea-ice growth 

Bishakhdatta Gayen, Ankit Bhadouriya, Alberto Naveira Garabato, and Alessandro Silvano

Antarctic sea ice plays a critical role in regulating heat and gas exchanges between the atmosphere and the Southern Ocean by insulating the upper-ocean mixed layer. During winter, sea ice formation drives vertical mixing, deepening the mixed layer and entraining subsurface heat that feeds back on subsequent ice growth. Recent years have seen an alarming decline and increased variability in Antarctic sea ice. This trend highlights the urgent need to better understand and represent the processes controlling ice growth in predictive models. Despite its importance for climate projections, this coupled ice–ocean feedback remains poorly constrained because wintertime observations are sparse. Here, we use high-resolution, state-of-the-art large-eddy simulations to identify a previously unrecognized process in the Southern Ocean: overshoot convection. We show that sea ice formation generates energetic, meter-scale saline plumes that penetrate beyond the mixed layer and overshoot into the pycnocline. These plumes rebound upward, entraining warmer subsurface waters associated with Circumpolar Deep Water back into the mixed layer and enhancing upward heat fluxes that moderate further ice growth. Recent years have seen an alarming decline and increased variability in Antarctic sea ice, underscoring the urgency of improving the representation of such processes in predictive models. We develop a theoretical framework to quantify plume-driven heat fluxes and apply it to an ice–ocean multi-year reanalysis dataset over the recent decade, demonstrating the large-scale relevance of overshoot convection. Our results indicate that this process limits Antarctic sea ice growth and spatial expansion, providing a physical explanation for observed regional variations in ice thickness. Crucially, overshoot convection is absent from current climate-scale models, highlighting a key missing process in projections of future Antarctic sea ice evolution and climate change.

How to cite: Gayen, B., Bhadouriya, A., Naveira Garabato, A., and Silvano, A.: Overshooting convective plumes and their role in winter Antarctic sea-ice growth, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15536, https://doi.org/10.5194/egusphere-egu26-15536, 2026.

EGU26-17515 | ECS | Orals | CR3.1

Advancing Arctic summer sea ice freeboard from ICESat-2 

Isolde Glissenaar, Jack Landy, Wenxuan Liu, and Ellen Buckley

The ICESat-2 laser altimeter was launched in 2018 and has been measuring surface elevation used to determine sea ice thickness. The sea ice freeboards during winter (November-April) show strong agreement with in-situ observations. However, meltwater ponds accumulating on the sea ice over summer have prevented generating valid sea ice thickness observations from ICESat-2 in the summer months. Melt ponds hinder the classification of lead surfaces, leading to errors in the sea surface reference.

Utilizing more than 80 Sentinel-2 optical images coinciding within 5 minutes with ICESat-2 tracks, we have trained a Gaussian Mixture clustering algorithm that correctly classifies laser returns throughout the melt season. On testing images, the newly developed classification performs considerably better than the ATL07 classification, which was designed to be applied over winter conditions. The new classification was used to create an ICESat-2 summer laser freeboard dataset. The freeboards were validated with NASA's summer airborne lidar data acquisition campaign over July 2022.

The new summer freeboard dataset captures the melt season well, showing a quick decrease in freeboard during the melt of the snowpack in May and June and a slight increase at the start of autumn in September.

The summer sea ice freeboard dataset from ICESat-2 provides promising opportunities to calculate year-round sea ice thickness and volume, improve seasonal predictability, validate and improve the representation of sea ice in coupled climate models, and improve shipping risk assessment. 

How to cite: Glissenaar, I., Landy, J., Liu, W., and Buckley, E.: Advancing Arctic summer sea ice freeboard from ICESat-2, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17515, https://doi.org/10.5194/egusphere-egu26-17515, 2026.

We report on a novel data set of the melt-pond fraction on Arctic sea ice. Melt ponds on Arctic sea ice are an important phenomenon of the summer-melt process. They reduce the surface albedo of sea ice substantially, by that influence the net shortwave radiation balance, and with that the amount of solar radiation energy that is received by the sea ice-ocean system in the Arctic during summer. This has also implications for under-ice biogeochemical processes and ice mechanics. Melt ponds increase the uncertainty in the sea-ice concentration retrieved from satellite microwave radiometer measurements. Melt ponds have been observed by a number of satellite sensors, mostly in the optical and near-infrared wavelength range. Here we present an updated version of a spectral un-mixing approach published earlier that led to a data set of melt-pond fraction on Arctic sea ice with 8-daily sampling for months May through August from 2000 through 2011. The approach is based on reflectance measurements of channels 1, 3 and 4 of the Moderate Resolution Imaging Spectroradiometer (MODIS) on board the Earth Observation Satellite (EOS) Terra satellite. We modified the approach and derived the daily melt-pond fraction on Arctic sea ice at 500 m and at 12.5 km grid resolution for months June through August from 2000 through 2024 from MODIS v6.1 observations. In addition, we provide the net ice surface fraction – aka the fraction of sea ice without melt ponds – and the fraction of open water between the ice floes. We performed an evaluation of our data set against various independent observations. Our MODIS melt-pond fraction agrees within -3 % to +4 % with independent estimates of the melt-pond fraction from very-high resolution optical satellite imagery and from Operation Ice Bridge Digital Camera System imagery. The MODIS open-water fraction is smaller by 2 % to 6 % than that from independent estimates. The net ice-surface fraction tends to be larger by 2 % to 9 % than that from independent estimates. The 12.5 km gridded product shows a slightly worse (by 1 %) agreement. While our 12.5 km gridded MODIS product under-estimates the melt-pond fraction from very-high resolution optical satellite imagery by about 2 % in the mean (median: 3 %), the Medium Resolution Imaging Spectrometer (MERIS) product over-estimates these independent estimates by about 8 % (median: 9 %). Our MODIS melt-pond fraction data set is available from Sadikni and Kern (2025): https://doi.org/10.25592/uhhfdm.18069.

How to cite: Kern, S. and Sadikni, R.: 25-years of summer-time daily melt-pond fraction on Arctic sea ice derived from TERRA-MODIS sensor measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17914, https://doi.org/10.5194/egusphere-egu26-17914, 2026.

EGU26-18290 | Orals | CR3.1

Sea ice and snow six years after MOSAiC: bringing data to numerical models 

Polona Itkin, Jari Haapala, and Glen E. Liston

MOSAiC expedition in 2019/2020 collected an unprecedented volume of sea ice and snow data. For example, over 50 autonomous drifters, more than 160 km of sea ice thickness transect lines, nearly 250 snow pits, hundreds of satellite images, and thousands of ship radar images. Studies based on these data have yielded, among others, new data-based estimates of snow thermal conductivity, discovered new freezing mechanisms in the ridges and pinned the limits of sea ice deformation scale invariance. MOSAiC data analyses show that the snow depth and ice thickness was largely ice-age independent and that most of the winter’s snow was trapped in the deformed ice and that the loss of snow to leads was small.

Numerous sea ice deformation events formed the rough topography that trapped the snow throughout the winter. In order to better understand these processes and interactions, drifter, satellite remote sensing, and ship radar data can be used to analyse the deformation processes themselves, including reactivation of the leads and pressure ridges. These dynamics can not be represented in continuum models due to the spatial scale discrepancy. Here we will present how the sea ice deformation data from remote sensing can be used to create ice topography to constrain the snow distribution processes and, with it, the ice growth. We will use the recently developed methodology of data-model fusion by Itkin and Liston (2025, The Cryophere) to quantify the local snow-ice processes on spatial extents relevant also to the continuum models.

How to cite: Itkin, P., Haapala, J., and Liston, G. E.: Sea ice and snow six years after MOSAiC: bringing data to numerical models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18290, https://doi.org/10.5194/egusphere-egu26-18290, 2026.

EGU26-438 | ECS | Posters on site | CR3.2

Sharper Resolution of Arctic Sea Ice Dynamics with Non-Conforming Finite Elements in FESOM2 

Jan Gärtner and Sergey Danilov

Sea ice dynamics in numerical models are discretized on a spatial grid, with variables located at grid cell vertices, edges, or centers. On triangular grids, the number of edges is three times larger than the number of vertices. Consequently, placing variables on edges --- corresponding to a non-conforming finite-element discretization --- increases the number of degrees of freedom and effectively enhances the spatial resolution on a given mesh. Idealized benchmark experiments without a coupled ocean using the CD-grid discretization, where sea ice velocity is placed on edges and tracers on vertices, have demonstrated an increased occurrence of small-scale fractures and more finely resolved features in the sea ice field compared to other discretizations. In this study, we present the first application of the CD-grid in a high-resolution, fully coupled sea ice--ocean simulation using FESOM2, using a spatial resolution in the Arctic of 4.5 km. We show that the CD-grid produces a more sharply resolved sea ice field with an increased occurrence of small-scale structures relative to the A-grid configuration, in which both velocity and tracers are placed on vertices, while maintaining the same large-scale sea ice characteristics. In addition, we present a scaling analysis of the CD-grid in parallel applications across varying core counts, including runtime benchmarks and a direct performance comparison with the A-grid.

How to cite: Gärtner, J. and Danilov, S.: Sharper Resolution of Arctic Sea Ice Dynamics with Non-Conforming Finite Elements in FESOM2, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-438, https://doi.org/10.5194/egusphere-egu26-438, 2026.

EGU26-483 | ECS | Posters on site | CR3.2

Implications of Numerical Error Growth in the Maxwell Elasto-Brittle Rheology for Sea Ice Fracturing and Spatial Heterogeneity 

Mirjam Bourgett, Martin Losch, and Mathieu Plante

The accurate simulation of sea ice deformation and fracturing remains a significant challenge, driving the development of advanced continuum rheologies. In particular, brittle (elasto-brittle or EB, Maxwell elasto-brittle or MEB, brittle Bingham-Maxwell or BBM) rheologies are a promising advancement, introducing a damage parameter that accounts for sub-grid scale fractures and material degradation under high stresses without requiring large deformations. They simulate realistic large scale fields with adequate heterogeneity and intermittency even at coarser resolution.

However, the conventional MEB implementation, which relies on correcting super-critical stresses to bind the simulated stress to the yield criterion, inadvertently introduces a growth of numerical errors in the stress field. These errors can be reduced by introducing the Plante and Tremblay (2021) generalized stress correction scheme.

Here, the generalized stress correction scheme is added to the implemenation of the MEB rheology in the sea ice component of the Massachussetts Institute of Technology general circulation model (MITgcm), a community model that also includes a viscous-plastic (VP) rheology.

The results of pan-Arctic simulations with different levels of numerical errors in the stress field are compared against simulations using the VP rheology to identify the effect of numerical errors on the deformation behaviour. Our findings reveal three critical insights. First, we find that the generalized correction scheme successfully reduces numerical errors in the stress field in the complex Arctic simulations. Second, we show that reducing the numerical errors effectively reduce the number of simulated Linear Kinematic Features (LKFs). This confirms that numerical errors are partly responsible for the generated spatial heterogeneity in the MEB rheology. Third, we introduce artificial numerical errors to the yield curve of both MEB and VP to find that the MEB rheology is a lot more sensitive to it than the VP rheology. Additionally, we use idealized scenarios to isolate the problem from the complexitiy of an Arctic simulation. In the idealized experiments we can reproduce our results and find that the fracture angle seems to be dependent on the generalized correction scheme, as well.

Our work leads to more understanding of the MEB rheology with the goal of finding the source of heterogeneity and the seeding of LKFs in sea ice models. 

How to cite: Bourgett, M., Losch, M., and Plante, M.: Implications of Numerical Error Growth in the Maxwell Elasto-Brittle Rheology for Sea Ice Fracturing and Spatial Heterogeneity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-483, https://doi.org/10.5194/egusphere-egu26-483, 2026.

EGU26-599 | ECS | Posters on site | CR3.2

Deep Arctic Ocean Warming Enhanced by Heat Transferred from Deep Atlantic 

Ruizhe Song, Xianyao Chen, Hanwen Bi, Xiaoyu Wang, and Longjiang Mu

Observations since 1990s reveal widespread warming in the deep and bottom Arctic Ocean. It is historically attributed to geothermal heating, whereas the impacts of global and Arctic climate change on the deep and bottom Arctic Ocean warming remain unresolved. Our study demonstrates that during the recent decades, the Arctic Ocean deep water is warming at 0.020 ℃/decade in the Eurasian Basin between 2000 and 2600 m, exceeding what can be explained by geothermal heating. We find that the rapid warming in the deep Greenland Basin diminishes its cooling effect on the deep Eurasian Basin via the Fram Strait, leading to the warming in the deep Eurasian Basin. Meanwhile, the Lomonosov Ridge blocks this warming signal from reaching the deep Amerasian Basin, maintaining its relative slow warming rate of 0.003 ℃/decade. Our findings indicate that the deep Greenland Basin warming has already exerted obvious impacts on the deep Arctic Ocean.

How to cite: Song, R., Chen, X., Bi, H., Wang, X., and Mu, L.: Deep Arctic Ocean Warming Enhanced by Heat Transferred from Deep Atlantic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-599, https://doi.org/10.5194/egusphere-egu26-599, 2026.

EGU26-2833 | ECS | Posters on site | CR3.2

Biases in tropical Pacific teleconnections and ocean memory together limit spring sea ice predictability in dynamical models in the Weddell Sea 

Yuchun Gao, Yafei Nie, François Massonnet, Yongwu Xiu, Dániel Topál, Hao Luo, Xianqing Lv, and Qinghua Yang

Antarctic sea ice plays a critical role in modulating global climate variability and in supporting polar ecosystems. However, sea ice seasonal forecasts continue to show limited skill in capturing interannual variability across key regions and seasons. Here we evaluate seasonal predictions of Antarctic sea ice extent predictions from six Copernicus Climate Change Service forecast systems, focusing on the Weddell Sea, where springtime skill deteriorates rapidly with lead time. We identify two systematic sources of model error. First, models show excessive persistence of winter sea ice anomalies compared to observations, indicating an overdependence on ocean conditions. Second, they fail to adequately represent large-scale atmospheric circulation anomalies associated with El Niño–Southern Oscillation and Southern Annular Mode interactions, underestimating Amundsen Sea Low pressure anomalies and related wind patterns. These circulation-related biases appear to originate from misrepresented atmospheric responses to tropical Pacific sea surface temperatures. Our results prompt us to revisit sea-ice ocean couplings and better capture tropical-Antarctic teleconnections in dynamic models to improve Antarctic sea ice prediction.

How to cite: Gao, Y., Nie, Y., Massonnet, F., Xiu, Y., Topál, D., Luo, H., Lv, X., and Yang, Q.: Biases in tropical Pacific teleconnections and ocean memory together limit spring sea ice predictability in dynamical models in the Weddell Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2833, https://doi.org/10.5194/egusphere-egu26-2833, 2026.

EGU26-4488 | ECS | Orals | CR3.2

A Hybrid Neural Network-Finite Element Method for the Viscous-Plastic Sea-Ice Model 

Nils Margenberg and Carolin Mehlmann

We present an efficient hybrid Neural Network–Finite Element Method (NN-FEM) for the viscous–plastic (VP) sea-ice model used in climate simulations. VP solvers are costly due to the strongly nonlinear material law, with cost per degree of freedom increasing rapidly under mesh refinement. However, high resolution is needed to capture narrow deformation bands (linear kinematic features). Our approach enriches coarse-mesh FEM solutions with fine-scale corrections predicted by a locally applied neural network trained on high-resolution data. The patch-based network is small, parallelizable, and generalizes across right-hand sides and domains. Numerically, the method achieves comparable accuracy at approximately 11× lower cost and speeds Newton iterations by up to 10%.

How to cite: Margenberg, N. and Mehlmann, C.: A Hybrid Neural Network-Finite Element Method for the Viscous-Plastic Sea-Ice Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4488, https://doi.org/10.5194/egusphere-egu26-4488, 2026.

EGU26-6436 | Posters on site | CR3.2

End-to-end forecast of the Arctic sea ice initialised directly from observations 

Julien Brajard, Léo Edel, Cyril Palerme, Anton Korosov, and Laurent Bertino

We present IceCastNet, a data-driven model for forecasting Arctic sea ice state (including concentration, thickness, and drift) up to 10 days ahead. The model is trained on satellite-derived products: OSI-SAF for sea ice concentration and drift, and CS2SMOS for sea ice thickness. During the melt season, when CS2SMOS data are unavailable, the dataset is supplemented with the TOPAZ reanalysis. IceCastNet also uses meteorological forecasts (10-meter wind and 2-meter air temperature) from ECMWF as forcing.

The architecture is based on a graph-transformer design, similar to that used in the Artificial Intelligence/Integrated Forecasting System (AIFS), and implemented within ECMWF’s Anemoi framework. IceCastNet achieves skills comparable to, and in some cases better than, established baselines such as the operational TOPAZ system, particularly for sea ice concentration. These improvements appear to stem from reduced biases in initial conditions and lower forecast error. This is assessed by comparing IceCastNet outputs with debiased TOPAZ forecasts and independent sea ice concentration products, including SAR-derived estimates from the Danish Meteorological Institute (ASIP) and ice charts produced by experts at the U.S. National Ice Center.

The inference time for a 10-day forecast with IceCastNet of about 10 seconds is approximately two orders of magnitude shorter than that of physics-based systems such as TOPAZ. This substantial reduction in computational cost makes IceCastNet a computationally efficient alternative, although IceCastNet only provides the observed variables. Moreover, since it relies exclusively on operational, near-real-time data, IceCastNet is well-suited for integration into operational sea ice forecasting workflows.

The spatial resolution of IceCastNet forecasts follows that of the training data. We also show that applying a super-resolution procedure trained on high-resolution sea ice simulations from the model neXtSIM can enhance the resolution of IceCastNet outputs.

 

References:

CS2SMOS: https://doi.org/10.5194/tc-11-1607-2017
OSI-SAF: https://osi-saf.eumetsat.int/
AIFS: https://arxiv.org/abs/2406.01465
TOPAZ: https://doi.org/10.48670/moi-00001
ASIP: https://ocean.dmi.dk/asip/
neXtSIM: https://egusphere.copernicus.org/preprints/2025/egusphere-2024-3521/

How to cite: Brajard, J., Edel, L., Palerme, C., Korosov, A., and Bertino, L.: End-to-end forecast of the Arctic sea ice initialised directly from observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6436, https://doi.org/10.5194/egusphere-egu26-6436, 2026.

EGU26-7618 | ECS | Orals | CR3.2

GODAR: a new discrete element sea ice model 

Antoine Savard, Bruno Tremblay, and Arttu Polojärvi

Sea ice is a highly heterogeneous, granular material whose mechanical behavior arises from interactions among individual floes. This granular nature makes discrete element methods (DEMs) a natural choice for modeling sea ice dynamics. In principle, DEMs can resolve discontinuities, such as fractures and leads, and directly capture deformation, ridging, and dilatation processes without relying on parameterizations. However, several challenges (e.g., contact detection, floe geometry, open water treatment) limit their applicability to large-scale simulations. For these reasons, computational efficiency, and historical precedent, continuum models have long been the community’s choice for simulating sea ice at larger scales, even though they face their own challenges. Although running high-resolution (<2 km) state-of-the-art continuum models improves the representation of linear kinematic features (LKFs) and deformation statistics, this is computationally expensive, and Earth system models running at coarser resolutions can’t benefit from this. Thus, they are supplemented with parameterizations to account for subgrid-scale processes that cannot be captured by rheological models alone. Therefore, a modeling framework that bridges the gap between particle-resolving and continuum scales is required.

We present a new sea ice discrete element model, the Granular flOe Dynamics for seA ice Rheology (GODAR) model, to bridge the gap between the engineering and pan-Arctic scales. The purpose of this model is to support the development of parameterizations representing the granular behavior of sea ice in continuum sea ice models. GODAR includes a ridging parameterization, a rolling-resistance model that captures complex geometries, and a novel sheltering parameterization. The model explicitly resolves the formation and evolution of LKFs and reproduces the dilatant behavior observed in granular materials, while maintaining computational tractability suitable for regional domains by using cylindrical particles. Results from shear experiments demonstrate that ridges are highly localized along the failure planes and that the ridge build-up coincides with a positive angle of dilatancy (compressive regime). The novel geometric sheltering coefficient can reduce the total form drag of the sheltered floes, resulting in a non-zero moment on assemblies of floes. Finally, GODAR could be easily improved to run basin-scale simulations in the near future, and be extended to a seamless model capable of representing all ice types – sea ice, icebergs, ice shelves, and land ice – within a unified framework.

How to cite: Savard, A., Tremblay, B., and Polojärvi, A.: GODAR: a new discrete element sea ice model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7618, https://doi.org/10.5194/egusphere-egu26-7618, 2026.

EGU26-8940 | ECS | Orals | CR3.2

Application of discrete element methods to approximate sea-ice dynamics 

Saskia Kahl and Carolin Mehlmann

We present a hybrid approach to modelling sea-ice dynamics that integrates discrete elements to represent small-scale mechanical processes within large-scale simulations. Owing to resolution limitations in current climate models, these processes are typically poorly represented or neglected altogether in large-scale simulations. We extend the viscous–plastic model by introducing collision mechanics in a region of interest to capture elastic behaviour. To ensure a consistent, mass-conserving coupling between the continuum model and the discrete element method, sea-ice tracers are represented using Lagrangian particles. This enables a more accurate description of local dynamics. The hybrid approach allows phenomena such as ice jamming, which are difficult to capture with purely continuum-based models, to be simulated more accurately and at significantly reduced computational cost. It therefore provides an improved approach for understanding sea-ice dynamics and its role in the climate system.

How to cite: Kahl, S. and Mehlmann, C.: Application of discrete element methods to approximate sea-ice dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8940, https://doi.org/10.5194/egusphere-egu26-8940, 2026.

EGU26-9145 | ECS | Orals | CR3.2

Learning sea-ice physics from data: a hybrid ML-numerical modelling framework 

Nils Hutter, Alexander Wilms, and Stephan Juricke

Sea ice remains challenging to predict across spatial and temporal scales, from hourly floe-scale motion to seasonal regional forecasts and long-term climate projections. Increasingly complex numerical models have been developed to represent the strongly nonlinear dynamics and thermodynamics of sea ice, but their growing computational cost together with uncertainties in initial conditions and unresolved physical processes continues to limit their applicability. In recent years, machine-learning approaches trained on satellite observations or numerical model output have shown promise in predicting sea-ice evolution. However, while often accurate, such purely data-driven models provide limited physical interpretability, hindering the analysis of individual dynamic and thermodynamic processes and their response to climate change. Here we present a hybrid modelling framework that bridges these two approaches: a machine learning-enabled numerical sea-ice model. At its core is a differentiable implementation of a dynamic-thermodynamic sea-ice model in Python, which allows the computation of sensitivities with respect to model parameters as well as initial and boundary conditions. This enables systematic parameter optimization against observations and, more importantly, facilitates the replacement of individual parameterizations with lightweight machine-learning components. Once trained, these lightweight components remain physically interpretable due to their low complexity, explicit input-output relationships, and strictly local (pointwise) operation, in contrast to black-box, high-dimensional ML models. The hybrid model is embedded in an efficient data-loading infrastructure that provides access to diverse observational data sources, including satellite, buoy, and in-situ measurements, for training and evaluation. We demonstrate the capabilities of this framework by comparing alternative data-driven thermodynamic parameterizations for sea-ice and snow growth and melting rates trained on buoy and satellite data, and by assessing their impact on large-scale sea-ice evolution.

How to cite: Hutter, N., Wilms, A., and Juricke, S.: Learning sea-ice physics from data: a hybrid ML-numerical modelling framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9145, https://doi.org/10.5194/egusphere-egu26-9145, 2026.

EGU26-10536 | Orals | CR3.2

High-Resolution Sea Ice Drift Modelling Using Sentinel-2 and Discrete Element Method: Towards Subgrid Parameterization for Large-Scale Models 

Raed Lubbad, Biye Yang, Nick Hughes, Wenjun Lu, Sveinung Løset, and Wolfgang Dierking

Large-scale sea ice models still struggle to reproduce observed drift and deformation patterns, underscoring the need for physically based representations of unresolved floe-scale processes. Advances in high-resolution modelling and satellite imagery now offer new opportunities to investigate floe-scale dynamics and their influence on large-scale ice behaviour. These developments are essential not only for improving model fidelity but also for Arctic navigation and offshore safety.

As part of the ESA-funded HIRLOMAP project, we present a workflow for generating high-resolution sea ice products by integrating satellite observations, image processing, and numerical modelling. The study domain is a 110 × 110 km southeast of Svalbard. Two Sentinel-2 images (10 m resolution) acquired on 16th and 17th of April 2025 are used. Ice drift vectors were derived from the satellite images through feature tracking, enabling estimation of local displacement and deformation rates (divergence and shear).

To simulate ice dynamics, we employ a Discrete Element Model (DEM) with boundary conditions informed by satellite-derived drift. Environmental forcing includes wind fields from NORA3 and ocean currents from Barents-2.5, while ice thickness is obtained from CryoSat-2/SMOS products. The initial ice field is digitized from Sentinel-2 imagery, yielding around 40 000 floes. Computational efficiency is improved through hierarchical clustering and area-based filtering, reducing floe count to around 1 800 while conserving total ice concentration. Model calibration focuses on air drag coefficients to reproduce observed deformation patterns. Simulated drift and strain rates are compared against Sentinel-2 observations and Barents-2.5 outputs, demonstrating the capability of DEM to capture local-scale variability beyond continuum models.

Future work will address large-scale fracture processes (e.g., ridging), wave–ice interactions, strategies to enhance computational performance, and the integration of machine learning approaches to further advance modelling capabilities. Even though these processes are not yet included, the results presented here already demonstrate strong potential for delivering next-generation Arctic sea ice services that combine high-resolution satellite data and DEM-based modelling. Beyond its engineering applications, this approach demonstrates how DEM can act as a subgrid parameterization tool for continuum models, enabling large-scale systems to represent floe-scale processes such as deformation and fracture.

How to cite: Lubbad, R., Yang, B., Hughes, N., Lu, W., Løset, S., and Dierking, W.: High-Resolution Sea Ice Drift Modelling Using Sentinel-2 and Discrete Element Method: Towards Subgrid Parameterization for Large-Scale Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10536, https://doi.org/10.5194/egusphere-egu26-10536, 2026.

The Met Office GC5 climate model has a simple sea ice albedo. To improve this, new albedo schemes have been implemented for bare sea ice, snow on sea ice and melt ponds. These improved albedo schemes include a solar zenith angle dependence, a snow grain size dependence (for snow on sea ice) and a more scientifically accurate representation of absorption of sunlight within melt ponds.

Climate simulations of GC5 for present day and 2xCO2 have been performed with (and without) the improved sea ice albedo schemes. We will present the effect of improved sea ice albedos on the present climate and the effect when a doubling of CO2 has been imposed.

How to cite: Copsey, D.: New sea ice albedo schemes to be included in future Met Office climate models and their effect on the climate., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10773, https://doi.org/10.5194/egusphere-egu26-10773, 2026.

EGU26-11333 | ECS | Posters on site | CR3.2

neXtSIM-DG: The next-generation discontinuous Galerkin sea ice model 

Robert Jendersie, Einar Ólason, Timothy Spain, Thomas Richter, Tom Meltzer, Joe Wallwork, Aurélie Albert, and Nirav Vasant Shah

NeXtSIM-DG is a novel sea ice model developed as part of the Scale Aware Sea Ice Project (SASIP).
The continum model supports both the established viscous plastic rheology (mEVP) and the Brittle Bingham-Maxwell rheology (BBM). The discretization is based on higher-order discontinuous and continuous finite elements to accurately represent the sharp features of sea ice. Quadrilateral parametric meshes with regular topology are used to allow for easy coupling with ocean models and a highly efficient implementation.
Following best practices in software engineering, the C++ code is designed to be maintainable and easily extendable, with a modular design that allows users to add new physics implementations.
In this poster, we give an overview of neXtSIM-DG and present recent developments regarding its usability and performance. We demonstrate our model's heterogeneous compute capabilities, supporting shared-memory parallelization with OpenMP, full GPU acceleration through Kokkos and scaling across multiple CPUs via MPI.

How to cite: Jendersie, R., Ólason, E., Spain, T., Richter, T., Meltzer, T., Wallwork, J., Albert, A., and Shah, N. V.: neXtSIM-DG: The next-generation discontinuous Galerkin sea ice model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11333, https://doi.org/10.5194/egusphere-egu26-11333, 2026.

EGU26-13030 | ECS | Orals | CR3.2

A continuum visco-elasto brittle model for sea ice with a granular transition 

Anne-Sarah Amblard, Véronique Dansereau, and Jérôme Weiss

Sea ice is a complex material that exhibits various mechanical behaviors depending on its degree of fragmentation. In compact and largely intact regions, it behaves as a cohesive, damageable solid, a regime that is reasonably well represented by continuum visco-elasto-brittle models (Dansereau et al., 2016; Rampal et al., 2019, Olason et al., 2022). In contrast, where it becomes highly fractured and loose – such as within large linear kinematic features - it behaves as a frictional, decohesive granular media, a regime that is challenging to describe within a purely continuum framework. To better capture the transition between the two regimes in a visco-elasto-brittle framework, we introduce additional physical ingredients: a damage-dependence of the Poisson’s ratio, a damage-dependence of the cohesion and a friction criterion.

We present results of a simple biaxial compression test in which each of these ingredients are included or not and demonstrate the strong interaction between their effect, highlighting the necessity of introducing them simultaneously to accurately reproduce the brittle to granular transition within sea ice.

How to cite: Amblard, A.-S., Dansereau, V., and Weiss, J.: A continuum visco-elasto brittle model for sea ice with a granular transition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13030, https://doi.org/10.5194/egusphere-egu26-13030, 2026.

EGU26-13276 | Posters on site | CR3.2

Distinct and synergistic influences of sea ice rheology and basal stress on the simulation of Arctic landfast ice 

Augustin Lambotte, Thierry Fichefet, François Massonnet, Laurent Brodeau, Pierre Rampal, Jean-François Lemieux, Frédéric Dupont, and Martin Vancoppenolle

Arctic landfast ice (LFI) is sea ice that remains mechanically immobilized along Arctic coastlines for prolonged periods. LFI influences the stability of the Arctic halocline by displacing coastal polynyas offshore and modifying the mixing of river plumes. In large-scale ocean–sea ice models, a realistic representation of Arctic LFI relies on two interacting modelling components: a grounding (basal stress) parameterization, which establishes anchor points in shallow waters, and the sea ice rheology, which controls ice deformation between these anchors. Here we examine the sensitivity of simulated Arctic LFI to these components and to their interaction. Simulations are performed using the Nucleus for European Modelling of the Ocean–Sea Ice Modelling Integrated Initiative (NEMO-SI³) platform on a 0.25° global grid. Two contrasting rheological formulations are considered: the adaptive elastic-viscous-plastic rheology with tensile strength (aEVPts) and the brittle Bingham-Maxwell rheology (BBM), each tested with and without a grounding scheme. Owing to its elastic component, BBM exhibits a more rigid mechanical behaviour than aEVPts and more readily immobilizes sea ice between anchor points, resulting in enhanced LFI formation. However, this increased rigidity of BBM also limits ice thickening in convergence zones, thereby reducing the effectiveness of the grounding scheme through a decrease in the number of anchor points. Comparison with in situ observations of Arctic LFI thickness further highlights the importance of accurately representing the timing and duration of sea ice immobilization. When sea ice becomes immobilized early and subsequently grows predominantly through thermodynamic processes, model biases in LFI thickness are significantly reduced, consistent with Stefan’s law for thermodynamic ice growth.

How to cite: Lambotte, A., Fichefet, T., Massonnet, F., Brodeau, L., Rampal, P., Lemieux, J.-F., Dupont, F., and Vancoppenolle, M.: Distinct and synergistic influences of sea ice rheology and basal stress on the simulation of Arctic landfast ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13276, https://doi.org/10.5194/egusphere-egu26-13276, 2026.

EGU26-13808 | ECS | Orals | CR3.2

A surprisingly capable minimal bonded discrete element model for sea ice 

Alexis Arlen, Earle Wilson, Véronique Dansereau, Yue (Olivia) Meng, and Ching-Yao Lai
Current climate models simulate sea ice as a continuous medium despite the discontinuities  arising from fracturing and floe-floe interactions. Discrete element models (DEMs) can directly resolve these discontinuities, making them valuable tools for understanding subgrid-scale sea ice dynamics. However, DEMs are typically limited by their high computational cost and large number of unconstrained microscale parameters, which hinder their validation and interpretability. In this work, we develop, calibrate, and evaluate the performance of a low-complexity, two-dimensional bonded DEM for process-based studies of ice flow and fracture. We modify the linear bonded particle model implemented in the molecular dynamics software, LAMMPS, to prevent failure in compression because unfractured sea ice is significantly stronger under compression than tension. Unlike most DEMs, our model does not explicitly integrate angular momentum, which halves the number of computations required for each particle. With this simplification, particles are frictionless and bonds do not break under torques. From simple shear experiments, we show that bonded elements behave elastically prior to failure, with an effective elastic modulus that scales linearly with the inter-particle bond stiffness. These experiments also illustrate that the ice deformation is localized in both space and time, in agreement with observations. Using a canonical geometry idealizing sea ice flow through the Nares Strait, we demonstrate that the model can reproduce ice arch formation and collapse previously observed in higher-complexity models. The small input parameter space can be explored with ensemble runs that would be infeasible for a higher-complexity model. We find that our model can represent four possible outcomes: viscous flow, ice arch formation and collapse, stable ice arch formation, and no fracturing. These regimes collapse onto a single control parameter given by the product of bond stiffness and critical strain. Despite neglecting key processes such as ridging and friction, our model reasonably represents short-timescale, discrete sea ice dynamics with fewer parameters to calibrate and lower computational cost than higher-complexity DEMs.

How to cite: Arlen, A., Wilson, E., Dansereau, V., Meng, Y. (., and Lai, C.-Y.: A surprisingly capable minimal bonded discrete element model for sea ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13808, https://doi.org/10.5194/egusphere-egu26-13808, 2026.

The horizontal size of a sea ice floe directly impacts both climatic feedbacks and sea ice dynamics. The floe size distribution (FSD) quantifies how the number of sea ice floes varies with floe size across a domain. The creation of models that can reproduce an accurate representation of the FSD is paramount for both climate prediction and seasonal Arctic forecasts, as floe size contributes to the ice-albedo feedback and sea ice evolution. Within the Community Ice CodE (CICE) sea ice model, sea ice floes are modelled using a prognostic FSD, where five processes may alter the FSD: lateral growth, lateral melt, new ice creation, welding (when two different floes coagulate), and wave fracture. Field notes have observed that when two floes weld together, the two floes may be bridged with younger ice providing an intermediary. We propose that the younger ice will be weaker, making the newly welded floe more likely to fracture. Yet CICE’s prognostic FSD carries no memory of prior welding or interactions, preventing the model from capturing this history-dependent weakness and how it influences dynamical processes, such as wave fracture or floe deformation. To account for this, we introduce a new parameterization for a floe’s health that calculates the fraction of floes in a given grid cell that have recently welded and that will be most susceptible to dynamic fragmentation. The parameterization also accounts for the effects of floes healing over time (with the welded bridge thickening), the effects of dynamic fracture on floe health, and the advection of the floe health metric through the model’s domain. With our accounting of floe health, we create a linear floe health dependent feedback that strengthens the influence of wave fracture and floe deformation. Finally, we use the new floe health metric to couple the FSD to CICE’s ice strength parameterization, weakening the ice in grid cells where many floes are the product of recent welding.

How to cite: Webb, G. and Bitz, C. M.: A new parameterization describing the health of a sea ice floe and its potential influence on wave fracture, ice deformation, and ice motion , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14808, https://doi.org/10.5194/egusphere-egu26-14808, 2026.

EGU26-16184 | ECS | Posters on site | CR3.2

Fracture of sea ice by ocean surface waves in CESM3 

Lettie A. Roach, David A. Bailey, Cecilia M. Bitz, Alice DuVivier, Marika M. Holland, Bruno Tremblay, and Geraint Webb

When ocean surface waves are present in ice-covered seas, they can cause sea ice to bend and fracture. Wave-induced fracture of sea ice could play an increasingly important role in the evolution of the Arctic and Antarctic sea ice covers. We present coupled simulations using the development version of the Community Earth System Model (CESM3) that now includes interactions between waves and sea ice, coupled via the sea ice floe size distribution. In particular, we show the influence of a unified sea ice fracture model based on elastic beam theory for the bending of a sea ice plate. This fracture model is valid for all wavelengths and spans the fully flexible and fully rigid limits, unlike previous approaches. Early results suggest that this model improves simulation of sea ice fracture and the floe size distribution, with implications for sea ice feedbacks. Further, we demonstrate a machine-learning-based emulation of the fracture scheme to reduce computational expense.

How to cite: Roach, L. A., Bailey, D. A., Bitz, C. M., DuVivier, A., Holland, M. M., Tremblay, B., and Webb, G.: Fracture of sea ice by ocean surface waves in CESM3, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16184, https://doi.org/10.5194/egusphere-egu26-16184, 2026.

EGU26-16686 | Posters on site | CR3.2

Using snow physical properties to constrain the ICEPACK sea ice model at McMurdo Sound, Antarctica 

Brian Anderson, Ruzica Dadic, Julia Martin, and Roberta Pirazzini

Snow on sea ice exerts strong controls on Antarctic sea ice thermodynamics and mass balance by modulating both radiative and conductive transfers in the surface energy budget. The high albedo of snow reduces absorbed shortwave radiation, while its relatively low but variable thermal conductivity insulates the ice, altering internal ice temperature gradients, growth rates and thus the timing and magnitude of basal heat flux to the ocean. Snow properties exhibit large spatial and temporal variability and assuming fixed snow-thermal parameters in models can bias conductive fluxes and the surface energy balance. For Antarctica in particular, thicker, storm-fed snowpacks modify vertical heat transfer. In this study we examine the influence of snow on Antarctic sea ice through the thermodynamics observed by three SIMBA bouys, which measure temperature at high spatial and temporal resolution through the snow and sea ice column. The three buoys were placed in locations with varying snow thickness (14cm, 2cm, 0cm). Using measurements of snow physical properties (thermal conductivity, surface temperature and roughness, snow grain radius, and albedo) to constrain the column physics model ICEPACK we examine the thermodynamics of the three sites. The results clearly indicate the influence of even very thin snow cover on sea ice, which makes internal sea ice temperatures much colder. The SIMBA bouy at the deeper snow site was maintained over two melt seasons and winter, and using this long time series shows that the model is most sensitive to variations in the key parameters of thermal conductivity and snow grain radius. These findings provide observationally grounded constraints on snow/ice thermodynamics that can improve sea ice models used in climate projections.

How to cite: Anderson, B., Dadic, R., Martin, J., and Pirazzini, R.: Using snow physical properties to constrain the ICEPACK sea ice model at McMurdo Sound, Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16686, https://doi.org/10.5194/egusphere-egu26-16686, 2026.

EGU26-22027 | Orals | CR3.2

A large-scale evaluation of sea-ice salt dynamics using new observations and NEMO-SI3 simulations 

Martin Vancoppenolle, Elise Ortega, Clément Rousset, Eva Lemaire, and Sébastien Moreau

Sea-ice salt dynamics control ice structure and ice–ocean salt fluxes, yet they remain weakly constrained at large scale and poorly evaluated in models. Here we compile a new global database of >1,200 sea-ice core salinity profiles and use it to provide the first large-scale evaluation of global 1° NEMO-SI3 simulations with new options for salt dynamics, including both state-of-the-art and historical reference parameterizations. The observations reveal a robust Arctic–Antarctic contrast: Antarctic sea ice is on average saltier and more variable, with differences expressed in the seasonal cycle, thickness space, and vertical structure, consistent with more frequent flooding and weaker flushing. Using this dataset, we systematically evaluate key model choices controlling salt dynamics, including prognostic versus diagnostic vertical salinity, gravity-drainage parameterizations, and the new-ice liquid fraction. With appropriate parameter settings, the model reproduces observed hemispheric contrasts, vertical profiles, and salinity–thickness relationships, while highlighting larger uncertainties and process gaps in Antarctic salt dynamics.

How to cite: Vancoppenolle, M., Ortega, E., Rousset, C., Lemaire, E., and Moreau, S.: A large-scale evaluation of sea-ice salt dynamics using new observations and NEMO-SI3 simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22027, https://doi.org/10.5194/egusphere-egu26-22027, 2026.

EGU26-458 | ECS | Orals | OS1.9

Fully polarimetric dual-frequency radar monitoring of Arctic sea ice 

Maisha Mahboob and Mallik Mahmud

The NASA–ISRO SAR (NISAR) mission will provide the first spaceborne dual-frequency (L- and S-band) radar observations of polar regions, which is capable of acquiring fully-polarimetric acquisitions. While L-band polarimetric capabilities are relatively well understood from previous missions and airborne campaigns, the S-band component represents a novel observational opportunity whose potential for sea ice characterization remains largely unexplored. Because of the fast changing sea ice regime in the Arctic, there is a growing need to understand what observational capabilities emerging synthetic aperture radar (SAR) system can offer for sea ice monitoring.

This study leverages very high resolution airborne UAVSAR imagery at fully-polarimetric mode from winter and summer seasons in the Beaufort Sea to investigate how dual-frequency SAR can provide separability of thinner sea ice classes over the annual thermodynamic cycle. We examine SAR backscatter and a range of parameters derivable from fully-polarimetric data to assess their utility in ice type discrimination.

Given S-band's intermediate wavelength between L-band and C-band, we anticipate distinct scattering behavior arising from its sensitivity to ice properties at scales different from those of established frequencies. This study aims to characterize how L- and S-band respond to varying ice conditions across seasons and to explore whether the two frequencies offer complementary information for ice classification. Also, we would like to develop a ranking for most efficient parameters from separability matrices. These findings will inform the development of sea ice monitoring frameworks for the imminent NISAR era.

How to cite: Mahboob, M. and Mahmud, M.: Fully polarimetric dual-frequency radar monitoring of Arctic sea ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-458, https://doi.org/10.5194/egusphere-egu26-458, 2026.

EGU26-2593 | ECS | Orals | OS1.9

Canadian Lake Ice Cover in the Early 21st-Century 

Justin Murfitt and Claude Duguay

Lake ice cover is a key component of the Earth’s cryosphere system. The absence of lake ice can have important implications for local energy budgets and influence the occurrence of extreme weather events, such as lake-effect snow systems. Additionally, ice formation is critical in the establishment of ice road transportation networks in areas such as Northern Canada, which allow for the transportation of goods and people during winter months. Within the WMO’s Global Climate Observing System (GCOS) Lakes Essential Climate Variable (ECV), lake ice has been identified as a key indicator for monitoring climate change. While long-term ground-based records of lake ice exist, the quantity of these measurements has declined, and over the last two decades, remote sensing has become increasingly relied on to provide information about global lake ice conditions. This is reflected in the multitude of operational lake ice products now available, including: the Multisensor Snow and Ice Mapping System (IMS), the MODIS Snow and Ice Cover, ESA Lakes CCI+ Lake Ice, and the Copernicus Land Service Lake Ice Extent products. These products exhibit different advantages and disadvantages related to the quality of retrievals, number of lakes/spatial resolution, and temporal coverage, which can limit their application for real-time monitoring or understanding of changes in lake ice conditions for smaller lakes.

This presentation will showcase a new operational product, specifically focused on providing daily lake ice coverage for lakes in Canada larger than 2.25 km2. The product is adapted from the processing chain utilized for the generation of the ESA CCI+ Lake Ice Cover Product but includes data for more than 36,000 lakes (500 m grid). The product is derived from over 1.5 PB of MODIS optical data and captures variation in the ice coverage during the two most recent decades (2000 – 2023). This presentation will describe and discuss the general trends and spatial patterns in lake ice cover across Canada, with connections to recent temperature trends. Additionally, an application of the product for monitoring ice roads will be highlighted by showcasing how the resolution of the product can be used to evaluate the timing of ice cover for lakes along key identified ice routes, such as the Tibbit to Contwoyto, Wekweèti, and Gamèti winter roads.

How to cite: Murfitt, J. and Duguay, C.: Canadian Lake Ice Cover in the Early 21st-Century, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2593, https://doi.org/10.5194/egusphere-egu26-2593, 2026.

Since the previous Japanese Arctic projects (ArCS and ArCS II projects), we have accumulated and evaluated scientific data, providing knowledge to the Joint Program for Scientific Research and Monitoring (JPSRM) established under the Central Arctic Ocean Fisheries Agreement (CAOFA). This knowledge could form the basis for conserving and utilizing marine resources. Here, contributions of the Japanese Arctic studies to the CAOFA JPSRM Implementation Plan are presented. During the 2020 R/V Mirai cruise in collaboration with the Synoptic Arctic Survey (SAS), unusually low oxygen and acidified water was found on the Chukchi Borderland (CBL), a high-seas fishable area of the Pacific Arctic. The integrated SAS data suggested that Beaufort Gyre shrinkage and Atlantification triggered a frontal northward flow along the CBL that transported the low oxygen and acidified water from the shelf-slope north of the East Siberian Sea. Therefore, the CBL area should be monitored as a bellwether of ecosystem degradation caused by ocean acidification and deoxygenation in the Central Arctic Ocean. This finding was cited in the CAOFA JPSRM Implementation Plan, and is proposing a most urgent monitoring site, which is at risk of ocean acidification and deoxygenation, in the Agreement Area. Future contributions to the CAOFA JPSRM are expected through the scientific surveys that will be conducted by the Japanese new icebreaker, Arctic Research Vessel (ARV) Mirai II.

How to cite: Nishino, S.: Japanese Arctic projects’ contributions to the Central Arctic Ocean Fisheries Agreement, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2619, https://doi.org/10.5194/egusphere-egu26-2619, 2026.

EGU26-2981 | ECS | Posters on site | OS1.9

The impact of climate change on Arctic acidification 

Chenglong Li

The Arctic Ocean experienced severe acidification in the subsurface layer owing to the increased invasion of Pacific Winter Water. However, the recent development and its control mechanisms remain unclear. Here we show that the subsurface acidifying waters (aragnite undersaturation) have further expanded northward, while it has been significantly thinned and shallowed in the western Canada Basin since 2015, in contrast to the thickening and deepening of the acidifying waters during 1994-2015. In the Northern Canada Basin, the more acidic waters in subsurface were also expanded substantially, which is mainly enhanced by the local enhancement of primary production in surface layer due to rapid sea ice loss.

How to cite: Li, C.: The impact of climate change on Arctic acidification, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2981, https://doi.org/10.5194/egusphere-egu26-2981, 2026.

EGU26-3566 | ECS | Posters on site | OS1.9

Potential for future erosion in the Arctic in the CANARI HadGEM3 large ensemble 

Stefanie Rynders and Yevgeny Aksenov

The presence of sea ice at the coast prevents coastal erosion of permafrost in the Arctic most of the year. Decreasing sea ice due to climate change will extend the erosion season. We examine coastal ice presence in a single model large ensemble future projection under the SSP3.70 scenario. We compare sea ice presence against locations with favourable geological conditions for erosion. The Arctic Ocean circulation pattern determines whether nutrients from erosion will be retained in the Arctic or end up the North Atlantic. Both sea ice and circulation conditions depend on the large scale atmospheric pattern, therefore we examine the correlation between high erosion conditions and enhanced outflow conditions. The contributions of Rynders and Aksenov were supported by the National Capability Multicentre Round 2 funding from the Natural Environment Research Council (BIOPOLE grant no. NE/W004933/1 and CANARI grant no. NE/W004984/1).

How to cite: Rynders, S. and Aksenov, Y.: Potential for future erosion in the Arctic in the CANARI HadGEM3 large ensemble, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3566, https://doi.org/10.5194/egusphere-egu26-3566, 2026.

EGU26-4435 | Orals | OS1.9

Resolved boundary currents at high resolution contribute to stronger future ocean convection in the Arctic 

Ruijian Gou, Haichao Guo, Yingjie Liu, Gerrit Lohmann, and Lixin Wu

Observational evidence indicates enhanced ocean convection near the sea ice edge in the Nordic Sea. However, whether sea ice retreat in a warming climate would further strengthen convection remains uncertain. Using a high-resolution climate model and comparing it with a low-resolution version, we find a more pronounced future increase in convection in the Arctic Ocean. A key reason for this difference is that at higher resolution, resolved boundary currents transport high-density Atlantic water more efficiently toward high latitudes along the ocean boundary. As sea ice retreats and low-density freshwater input diminishes, the high-density water can no longer subduct. Meanwhile, surface currents strengthen more than deeper currents, and the resulting shear weakens stratification before heat loss occurs. Our study suggests that future ocean convection and ventilation in the Arctic Ocean may be stronger than present projections from low-resolution models indicate.

How to cite: Gou, R., Guo, H., Liu, Y., Lohmann, G., and Wu, L.: Resolved boundary currents at high resolution contribute to stronger future ocean convection in the Arctic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4435, https://doi.org/10.5194/egusphere-egu26-4435, 2026.

EGU26-4497 | ECS | Posters on site | OS1.9

Study on the Mechanisms and Predictability of Beaufort Sea Ice Retreat: Insights from Ocean-Ice Model and Remote Sensing 

Zijia Zheng, Hongtao Nie, Shuo Wei, Wei Zhao, and Xiaofan Luo

The Beaufort Sea has experienced significant sea ice retreat in recent decades, driven by both thermodynamic and dynamic processes. This study investigates the drivers and predictability of summer sea ice retreat in the Beaufort Sea by integrating an ocean–sea ice model with satellite-derived sea ice concentration data and atmospheric reanalysis products. Model diagnostics from 1994 to 2019 reveal that thermodynamic processes dominate annual sea ice loss (approximately 90%), with vertical heat flux accounting for roughly 85% of total oceanic heat input. The summer sea ice minimum area and the day of opening, derived from either model results and satellite observations, have a strong correlation with R² = 0.60 and R² = 0.77, respectively, enabling regression equations based solely on remote sensing data. Further multiple linear regression incorporating preceding winter (January to April) accumulated temperature and easterly wind yields moderately robust forecasts of minimum sea ice area (R² = 0.49) during 1998–2020. Additionally, analysis of reanalysis wind data shows that the timing of minimum sea ice area is significantly influenced by the frequency and intensity of sub-seasonal easterly wind events during melt season. These results demonstrate the critical importance of remote sensing in monitoring Arctic sea ice variability and enhancing seasonal prediction capability under a rapidly changing climate.

How to cite: Zheng, Z., Nie, H., Wei, S., Zhao, W., and Luo, X.: Study on the Mechanisms and Predictability of Beaufort Sea Ice Retreat: Insights from Ocean-Ice Model and Remote Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4497, https://doi.org/10.5194/egusphere-egu26-4497, 2026.

EGU26-4781 | Orals | OS1.9

The Influences of Surface Waves on the Modeling of Arctic Sea Ice 

Jingkai Li and Yizhi Wang

Under ongoing global warming, Arctic sea-ice extent and thickness have declined markedly in recent decades, while open-water area has expanded. One immediate consequence is an intensification of wave activity due to enlarged fetches, which in turn strengthens wave–ice interactions. Compared with the understanding of ice impacts on waves, the response of sea-ice evolution to wave effects remains less well constrained—particularly from a basin-scale, climatological perspective. Here, using the Los Alamos sea-ice model (CICE), we incorporate four wave-related processes — Stokes drift, wave radiation stress, wave-induced mixing, and wave-induced fracture — and conduct a 10-yr simulation to quantify both the individual and combined impacts of these processes on Arctic sea-ice states. The results show that there are seasonal variations in the influence of ocean waves on sea ice concentration. However, the variations in modeled sea ice volume are not always the same for each year both qualitatively and quantitatively. In terms of the degree of influence, wave-induced ice fracture has the strongest influence on summer, autumn, and annual average sea ice concentration. But for specific periods and sea areas, the mechanism with the greatest influence may vary.

How to cite: Li, J. and Wang, Y.: The Influences of Surface Waves on the Modeling of Arctic Sea Ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4781, https://doi.org/10.5194/egusphere-egu26-4781, 2026.

EGU26-5839 | Orals | OS1.9

Towards an Early Warning System for Arctic Freshwater-Driven Tipping Points in the Greenland Ice Sheet and North Atlantic Subpolar Gyre with AEROSTATS 

Christine Gommenginger, Adrien C. H. Martin, David McCann, José Marquez Martinez, Samantha Lavender, Dougal Lichtman, Christian Buckingham, Alice Marzocchi, Thomas Prime, Louis Clément, Simon Josey, and Jeremy Grist

The climate system is approaching dangerous tipping points, with the potential collapse within decades of critical components such as the Greenland Ice Sheet and the North Atlantic Subpolar Gyre posing severe risks to European weather and global climate stability. Changes in Arctic freshwater, driven by changes in ice-sheet and sea-ice melt and atmosphere-ocean-ice interactions, play a central role in these risks by influencing ocean stratification, deep water formation and air-sea fluxes. Despite the urgent need for early warnings, major gaps remain between existing observations and the data required to constrain predictive models, limiting confidence in future projections.

Earth-orbiting satellites and in situ observations provide essential information on large-scale ocean, cryosphere, and atmosphere change, but they struggle to capture fast processes at kilometre and sub-kilometre scales in complex regions such as marginal ice zones. A different type of observations is needed to quantify the role of these processes in exchanges of freshwater, heat, and momentum that the Arctic and the Greenland Ice Sheet to the North Atlantic Subpolar Gyre.

This paper will introduce AEROSTATS (Aerial Experimental Remote sensing of Ocean Salinity, heaT, Advection, and Thermohaline Shifts), a UK-led international project designed to demonstrate a new approach to long-term, low-cost, low-carbon monitoring of Arctic freshwater processes in Greenland’s dynamic ocean–ice margins. AEROSTATS focuses on innovative airborne platforms capable of remote, high-resolution imaging of total surface current vectors, near-surface winds, sea surface salinity, ocean colour, and sea surface temperature at 1-10km and sub-daily scales.

Funded as a high-risk, forward-looking project, AEROSTATS seeks to collect and integrate data from new airborne instruments, in situ surface and subsurface platforms, spaceborne sensors, and high-resolution reanalyses and models. A core element is a 2028 year-round field campaign in the Greenland/Subpolar Gyre region deploying airborne systems to observe freshwater-driven processes across seasons. By combining multi-platform observations with models and reanalyses using digital tools such as machine learning and digital twins, AEROSTATS aims to establish new long-term monitoring capability to substantially improve early warning for freshwater-related tipping points.

How to cite: Gommenginger, C., Martin, A. C. H., McCann, D., Marquez Martinez, J., Lavender, S., Lichtman, D., Buckingham, C., Marzocchi, A., Prime, T., Clément, L., Josey, S., and Grist, J.: Towards an Early Warning System for Arctic Freshwater-Driven Tipping Points in the Greenland Ice Sheet and North Atlantic Subpolar Gyre with AEROSTATS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5839, https://doi.org/10.5194/egusphere-egu26-5839, 2026.

EGU26-6365 | ECS | Orals | OS1.9

A strengthening dipole pattern in Arctic Ocean dynamics observed by GRACE/GRACE-FO 

Yunju Chae, Ki-Weon Seo, and SungHyun Nam

The Arctic Ocean has changed rapidly over recent decades as sea ice has declined, freshwater inputs have increased, and atmosphere–ocean coupling has evolved. Yet the resulting basin-scale variability in ocean mass remains poorly constrained because in situ observations are sparse and satellite altimetry is limited at high latitudes. Here we use satellite gravimetry from GRACE and GRACE-FO to quantify Arctic Ocean bottom pressure (OBP) variability from 2002 to 2024, providing a direct measure of mass redistribution that is independent of steric effects. To isolate dynamic ocean signals, we remove land leakage and eustatic contributions using a forward-modeling framework that accounts for self-attraction and loading. Empirical Orthogonal Functions (EOF) analysis of the residual OBP field reveals a leading-mode dipole pattern, with increasing ocean mass in the Beaufort Gyre region within the Canadian Basin and decreasing mass in the Kara Sea and Barents Sea. The corresponding principal component shows a robust strengthening over the two-decade record. While the underlying physical mechanisms warrant further investigation, the overall dipole structure is consistent with recent modeling studies suggesting intensified surface circulation under continued sea-ice loss. Overall, GRACE-derived ocean mass captures coherent, multi-decadal Arctic circulation change in a warming climate.

How to cite: Chae, Y., Seo, K.-W., and Nam, S.: A strengthening dipole pattern in Arctic Ocean dynamics observed by GRACE/GRACE-FO, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6365, https://doi.org/10.5194/egusphere-egu26-6365, 2026.

EGU26-6981 | ECS | Orals | OS1.9

Quantifying Pan-Arctic Freshwater Fluxes: A 20-Year Satellite-Based Daily River Discharge and Runoff Dataset 

Francesco Leopardi, Carla Saltalippi, Jacopo Dari, Luca Brocca, Peyman Saemian, Nico Sneeuw, Mohammad Tourian, and Stefania Camici

The Arctic region is undergoing a rapid and intense transformation driven by global climate change. Paradoxically, this coincides with a generalized decline in the density of hydrometric stations, resulting in fragmented spatiotemporal river discharge time series data that are insufficient to capture the complexity of ongoing dynamics. Under these challenging context, Arctic basins play a crucial role in regulating the freshwater budget, influencing ocean circulation and sea ice formation, and acting as a "litmus test" for the hydrological cycle's response to warming.

To address the scarcity of in-situ data, our work aims to provide continuous river discharge and runoff estimates at a daily scale and 0.25° spatial resolution for the entire continental Pan-Arctic region over the period 2003–2022. We employ STREAM model (SaTellite based Runoff Evaluation And Mapping; Camici et al., 2022), a semi-distributed conceptual hydrological model forced exclusively by temperature data and satellite observations, including precipitation, soil moisture, snow cover fraction, and Terrestrial Water Storage (TWS) anomalies from GRACE (Gravity Recovery and Climate Experiment) and its Follow-On mission (GRACE-FO). The integration of gravimetry data represents a key innovation—particularly relevant in the context of the future NGGM-MAGIC (Next-Generation Gravity Mission / Mass-change And Geophysics International Constellation) mission—as it enhances the characterization of hydrological processes in cold regions where TWS changes significantly drive river discharge and runoff variability. The model was first calibrated on 15 "donor" Arctic basins, achieving a median Kling-Gupta Efficiency index (KGE) of 0.80. To cover ungauged areas, we developed a regionalization framework based on aridity-index clustering, extending estimates to the entire Pan-Arctic domain. The resulting dataset was independently validated against 26 gauging stations and benchmarked against existing reanalysis products.

Results demonstrate that the regionalized model faithfully reproduces discharge seasonality and interannual variability over 70% of the Pan-Arctic area. Furthermore, trend analysis reveals statistically significant runoff trends in 18% of the domain, highlighting that the Pan-Arctic does not exhibit a uniform response to climate change, but rather diverse, localized reactions.

This work provides a consistent hydrological baseline based solely on satellite data, filling the gaps left by fragmented in-situ river discharge monitoring networks and offering a robust tool to investigate the interactions between climate change and hydrological extremes in the Pan-Arctic region, a critical climate hotspot.

How to cite: Leopardi, F., Saltalippi, C., Dari, J., Brocca, L., Saemian, P., Sneeuw, N., Tourian, M., and Camici, S.: Quantifying Pan-Arctic Freshwater Fluxes: A 20-Year Satellite-Based Daily River Discharge and Runoff Dataset, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6981, https://doi.org/10.5194/egusphere-egu26-6981, 2026.

EGU26-7485 | Posters on site | OS1.9

Properties and Effects of Mesoscale Eddies in the Eurasian Basin of the Arctic from a Model Simulation at 1-km Resolution 

Vasco Müller, Sergey Danilov, Thomas Jung, Nikolay Koldunov, and Qiang Wang

Mesoscale eddies are widespread in the Arctic Ocean affecting circulation, stratification, the transport of heat and salt, and consequently sea ice melt. We detect and track coherent eddies in a 1-km resolution Arctic Ocean simulation using the unstructured-mesh Finite volumE Sea ice-Ocean Model (FESOM2). Their spatial and seasonal distributions are analyzed, and quasi-3D eddy composites are used to quantify their influence on the water column, surface heat fluxes, and sea ice.

Eddy formation is highest along topographic features and the boundary current, with eddy sizes roughly corresponding to the local Rossby radius. Anticyclonic eddies are larger and more energetic than cyclonic eddies and can lift warm, saline Atlantic Water toward the surface, which increases the vertical heat flux and can cause localized basal sea ice melt. Cyclonic eddies, by contrast, mainly transport cold surface water downward and have little impact on the surface heat budget or sea ice. Edd-induced anomalies are strongest in Fram Strait, weaken downstream, and are larger beneath pack ice than in the marginal ice zone. These results are consistent with an eddy-ice pumping mechanism, where ocean-sea ice stress enhances vertical transport and contributes to eddy decay. Overall, the analysis shows that mesoscale eddies play an important role in the vertical exchange of heat in the Eurasian Arctic making them an important factor in the ongoing Atlantification of the Arctic Ocean. Since the role of eddies is expected to become even more important in the future, adequately representing them in model simulations will be necessary, despite the high resolution and computational cost required to resolve them.

How to cite: Müller, V., Danilov, S., Jung, T., Koldunov, N., and Wang, Q.: Properties and Effects of Mesoscale Eddies in the Eurasian Basin of the Arctic from a Model Simulation at 1-km Resolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7485, https://doi.org/10.5194/egusphere-egu26-7485, 2026.

EGU26-7957 | Posters on site | OS1.9

Ultra-high-resolution ocean-sea ice model: a new capability to simulate shelf-ocean processes 

Yevgeny Aksenov, Stefanie Rynders, Laura de Steur, Harle James, Ben Barton, Andrew Coward, Jeffrey Polton, and Ed Blockley

With much focus on the local and regional changes in the ocean and marine biogeochemistry, high-resolution ocean-sea ice models became a widely desired tool for ocean research.

We present analysis of the analysis of the kilometric scale resolution regional ocean model for the Arctic and North Atlantic developed at the National Oceanography Centre and aimed at resolving mesoscale circulation. The model ARC36 features NEMO ocean model coupled to the SI3 sea ice model [1].

To assess model performance and demonstrate its applicability to the regional assessments, the two case studies has been chosen: (1) the Western Fram Strait and the East Greenland Shelf and (2) the Svalbard. For these areas eddy dynamics has been analysed and compared to the mooring data and satellite imagery. We have also assessed exchanges between the fjords, the shelf and the open ocean.  The simulations are evident of fine structure in ocean currents and eddies, more detailed than in coarser resolution models. The model also simulates sea ice break-up at spatial scales from a few kilometres to several hundreds of kilometres, suggesting the usability of continuum sea ice models at high-resolution.

This work is funded by the Natural Environment Research Council (NERC) LTS-M Programmes CANARI (NE/W004984/1) and BIOPOLE (NE/W004933/1), by UKRI/NERC HighLight Topic Projects “Interacting ice Sheet and Ocean Tipping – Indicators, Processes, Impacts and Challenges (ISOTIPIC)”, by the grant NE/Y503320/1, and by the Met Office Advancing Arctic meteorological and oceanographic capabilities & services project, which is supported by the Department for Science, Innovation & Technology (DSIT), and uses the ARCHER2 UK National Supercomputing Service (https://www.archer2.ac.uk).

References

[1] Rynders, S., Aksenov, Y., Coward, A., and Harle, J.: First look at Arctic eddies in a kilometric NEMO5 simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7121, https://doi.org/10.5194/egusphere-egu25-7121, 2025.

How to cite: Aksenov, Y., Rynders, S., de Steur, L., James, H., Barton, B., Coward, A., Polton, J., and Blockley, E.: Ultra-high-resolution ocean-sea ice model: a new capability to simulate shelf-ocean processes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7957, https://doi.org/10.5194/egusphere-egu26-7957, 2026.

EGU26-9359 | Orals | OS1.9

Sea Ice classification in SWOT L3 products  

Anaëlle Treboutte, Gwenael Jestin, François Boy, Matthias Raynal, Sara Fleury, and Gerald Dibarboure

The launch of the altimetric satellite SWOT (Surface Water and Ocean Topography) was a revolution in oceanography and hydrology. With its120 km swath width, a spatial resolution of 500m² (in Low Resolution acquisition mode) and an instrumental random error significantly lower than the one from nadir altimetry, the Ka-Band Radar Interferometer (KaRIn) onboard SWOT mission also present a huge potential to develop applications in the polar regions. Indeed, the SWOT product  enables the observation of leads, icebergs and polynyas (Dibarboure and al 2024) through the measures of surface topography and backscatter coefficient.

 

The surface discrimination between leads and floes is the first step toward polar ocean monitoring, ice thickness and snow depth estimations. However because of the complexity of the surface (different surface roughness properties in the leads, presence of melt pounds) added to residual sensing errors (residual KaRIn random error, residual systematic errors, …) this first required achieved is not straightforward. Therefore several classification approaches were developed : one based on a statistical method (Markov Random Field), one based on an unsupervised machine learning method (Kmeans) and another one based on a supervised machine learning method (XGBoost). The objective of this paper is thus to present the results of these methods (their robustness, strengths and weaknesses) through local comparisons with respect to optical, SAR images and global comparison with existing state of the art products (OSISAF ice concentration products).

How to cite: Treboutte, A., Jestin, G., Boy, F., Raynal, M., Fleury, S., and Dibarboure, G.: Sea Ice classification in SWOT L3 products , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9359, https://doi.org/10.5194/egusphere-egu26-9359, 2026.

EGU26-9495 | Posters on site | OS1.9

Internal wave spectra and mixing in the warming Arctic 

Friederike Pollmann

The generation of internal wave generation might increase in the warming Arctic, especially at the sea surface, where wind power input into the upper ocean is substantially stronger as sea ice disappears. More internal wave energy implies stronger mixing that might lead to larger upward heat fluxes from the warm Atlantic Water, contributing to the ongoing sea-ice melt. To comprehensively test this hypothesis, a physics-based mixing parameterization building on an internal wave model that accounts for internal wave generation, propagation, and breaking, is required. To develop such a model, however, knowledge of the internal wave spectral characteristics and their spatio-temporal variability is indispensable. This study therefore investigates the vertical wavenumber spectra of internal wave energy and how their shape varies across the Arctic Ocean based on finescale hydrographic profiles collected by a variety of instrument platforms. It focuses on internal wave energy levels, vertical wavenumber spectral slope and bandwidth, and wave-driven mixing to elucidate their geographic and temporal variation and shed light on the environmental factors determining their variability.

How to cite: Pollmann, F.: Internal wave spectra and mixing in the warming Arctic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9495, https://doi.org/10.5194/egusphere-egu26-9495, 2026.

EGU26-12700 | ECS | Orals | OS1.9

A Multi-Tracer Study of Ventilation and Anthropogenic Carbon Storage in the Arctic Ocean 

Inigo Arnedo, Stanley Scott, Sophie Negele, Yannis Arck, Florian Meienburg, Niclas Mandarić, Alexander Junkermann, David Wachs, Núria Casacuberta Arola, Toste Tanhua, Markus Oberthaler, and Werner Aeschbach

The Arctic Ocean (AO) is a critical sink for anthropogenic carbon (Cant), sequestering emissions via intermediate and deep water formation, storing it for long periods of time. Understanding the timescales of these ventilation processes is essential for calculating the current inventory of Cant as well as predicting the AO’s capacity to store CO2 in a warming climate. However, observational constraints remain limited; while standard transient tracers (SF6, CFC-12) and other radionuclides successfully resolve surface and intermediate layers, they often fail to capture the older waters of the deep basins. Atom Trap Trace Analysis (ATTA) has opened a new way to measure deep ocean water residence times by using the radioactive noble gas 39Ar. Here we show the first fully resolved vertical profiles of Arctic ventilation and Cant using Transit Time Distributions (TTDs) derived from a novel combination of short-lived tracers and long-lived radioisotopes (39Ar, 14C). Their vertical distribution brings key information on ocean ventilation and hence the storage of anthropogenic carbon. We apply a Bayesian Inference framework to fit the TTD parameters from the different tracer data constraints.

We find that the mixing regime across the Nansen, Amundsen, and Makarov Basins is more advection-dominated than previously assumed in the deep basins. The profiles reveal that the Arctic stores up to 33% of its total Cant inventory below 1,500 m—vastly exceeding the global ocean average of ∼7%. While the deep Makarov Basin holds roughly half the carbon content of the Eurasian Basin, both reservoirs play a disproportionate role in deep sequestration. Conversely, we demonstrate that for the Atlantic Water Layer, which contains the bulk of the carbon, adding long-lived radioisotopes offers negligible improvement over standard tracers. These findings refine the Arctic carbon budget and highlight the necessity of adding long-lived radionuclides for constraining the deep ocean sink.

How to cite: Arnedo, I., Scott, S., Negele, S., Arck, Y., Meienburg, F., Mandarić, N., Junkermann, A., Wachs, D., Casacuberta Arola, N., Tanhua, T., Oberthaler, M., and Aeschbach, W.: A Multi-Tracer Study of Ventilation and Anthropogenic Carbon Storage in the Arctic Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12700, https://doi.org/10.5194/egusphere-egu26-12700, 2026.

EGU26-16244 | ECS | Orals | OS1.9

Role of Ice Rheology in Modulating Surface Stress and Sea-Ice Drift in the Beaufort Gyre 

Elizabeth Webb, David Straub, and Bruno Tremblay

The Beaufort Gyre is a prominent feature of Arctic Ocean circulation and a focal point for studies of Ekman dynamics. Midlatitude gyres are primarily forced by atmospheric winds, and Ekman pumping can be directly estimated from the atmosphere–ocean stress. However, in polar regions, the presence of sea ice modifies and mediates momentum transfer from the atmosphere to the ocean. In this context, the surface stress can be expressed as a weighted sum of atmosphere–ocean stress and ice–ocean stress, with the weighting determined by sea ice concentration. In regions of open water, the surface stress is dominated by direct atmospheric forcing, whereas in areas of high ice concentration it is largely controlled by the ice–ocean stress. Under these conditions, internal rheological stresses within the ice pack also play a role in redistributing the stress applied by the atmosphere before it is transmitted to the ocean. The combined action of surface and internal stresses determines the effective forcing felt by the ocean and has direct implications for Ekman pumping and the resulting circulation. To investigate the roles and influence of these stresses, we use output from the MIT general circulation model (MITgcm).

We begin with the free drift regime, in which internal rheological stresses are neglected, and assess the ability for this regime to produce sea ice drift. Observational data in the Arctic are limited, so we attempt to recover sea ice drift using readily available measurements, such as wind speed and altimeter derived sea surface height. Sea ice drift is first inferred from the balance between atmospheric and oceanic stresses, which captures the large scale features of motion reasonably well. Next, an iterative solver is applied to include the effects of Coriolis and sea surface tilt. Finally, comparison with the full rheology case shows that internal ice stress is necessary to reproduce the small scale features of ice motion. In regions of high ice concentration and during winter, rheological stresses become essential, and the free drift approximation no longer captures the observed motion.

Motivated by the limitations of the free drift approximation, the second part of this project examines how the presence of sea ice modifies the atmospheric stress transmitted to the ocean. In open water, wind stress acts directly on the ocean surface, whereas in ice covered regions the stress is applied to the ice and redistributed internally through rheological processes before reaching the ocean. Consequently, the stress experienced by the ocean differs from that applied at the surface. We analyze how internal ice stresses transform and redistribute atmospheric work across the ice pack, altering the effective surface stress and modulating Ekman pumping and ocean circulation within the Beaufort Gyre.

How to cite: Webb, E., Straub, D., and Tremblay, B.: Role of Ice Rheology in Modulating Surface Stress and Sea-Ice Drift in the Beaufort Gyre, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16244, https://doi.org/10.5194/egusphere-egu26-16244, 2026.

EGU26-17370 | ECS | Posters on site | OS1.9

A Decade of Arctic SSS Variability from Satellite and Reanalysis Data 

María Sánchez-Urrea, Marta Umbert, Martí Galí, Rebecca McPherson, Eva De Andrés, and Carolina Gabarró

The Arctic system is transitioning into a new regime whose properties are yet to be determined, as several feedback processes are undergoing unprecedented changes. Accelerated loss of sea ice and glaciers, enhanced discharge from major pan‑Arctic rivers, widespread permafrost degradation, and a strengthening of the global hydrological cycle are collectively reshaping the upper ocean, making it warmer and increasingly fresh. Sea Surface Salinity (SSS), recognized as an Essential Ocean Variable, provides an integrated measure of atmosphere-ice-ocean coupling. This work investigates the spatial and temporal patterns of SSS and their short-term evolution across nine pan-Arctic regions of the over the satellite period 2011–2022, with a particular focus on how these changes relate to key drivers of surface freshening. To achieve this, we use three Arctic-dedicated satellite products –two from ESA’s Soil Moisture and Ocean Salinity (SMOS) mission, developed by the Barcelona Expert Centre (BEC) and the Laboratory of Ocean and Climatology Expertise Center (LOCEAN), along with the Climate Change Initiative Salinity (CCI) dataset– and GLORYS12v1 model reanalysis. The consistent agreement between satellite observations and model outputs in September –when Arctic coverage is at its annual maximum (r > 0.54) –highlights recent advances in salinity retrievals and their ability to capture key oceanographic processes. Throughout this month, the spatial SSS trend revealed a statistically significant freshening in the northern Barents Sea, with particularly low anomalies in 2019 and 2022. On the other hand, a basin‑wide freshening is evident in all regions except the Kara Sea, with the largest declines (~0.2 yr⁻¹) found near major Arctic river mouths, where a concurrent SST increase further highlights the influence of continental freshwater inputs. The seasonal analysis over the year‑round ice‑free regions (Nordic and Barents Seas) revealed pronounced winter discrepancies among all products –including against in situ data– and most notably in the Norwegian Sea, showing that the drivers of these differences are not yet fully understood. A significant summer freshening emerged along southeastern Greenland, largely shaped by the pronounced anomalies of 2017 and 2021. These shifts reflect the combined influence of variability in sea‑ice export, the timing of melt onset, and atmospheric circulation patterns that govern the delivery and redistribution of freshwater. Meanwhile, the highest summer SSS anomaly in the Barents Sea occurred near the ice edge in 2015, following a winter with exceptionally large sea‑ice volume anomalies. The northward winter transport of sea ice (> 0.18 km³ month⁻¹), enhanced by a positive Arctic Oscillation phase, displaced the ice edge northward, leaving the meltwater signature above 77.5º N. These results highlight the crucial role of remotely sensed SSS in providing insights into the Arctic Ocean's changing conditions and their global implications.

How to cite: Sánchez-Urrea, M., Umbert, M., Galí, M., McPherson, R., De Andrés, E., and Gabarró, C.: A Decade of Arctic SSS Variability from Satellite and Reanalysis Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17370, https://doi.org/10.5194/egusphere-egu26-17370, 2026.

EGU26-17581 | Orals | OS1.9

Teleconnections in the ‘new Arctic’ 

Shengping He, Ke Fan, Jiazhen Zhao, Xinping Xu, and Jie Jiang

Rapid Arctic change is altering not only local climate conditions but also the teleconnections linking the Arctic to the midlatitudes. In the emerging “New Arctic,” characterized by strong summer sea-ice loss, expanded first-year ice, and deeper tropospheric warming, traditional Arctic–midlatitude linkages are being reshaped in both structure and strength. This study examines how these teleconnections are evolving using a combination of satellite observations, reanalysis data, and climate-model simulations. A key background change is the expansion of newly formed winter sea ice since the mid-1990s, increasing at about 0.6 million km² per decade. This growth is driven by enhanced autumn refreezing following intensified summer melt and is spatially concentrated over the central and eastern Arctic Ocean north of Siberia. Seasonally, the increase is dominated by November ice formation, highlighting the growing importance of late-autumn processes in the New Arctic.

Under this new background, several Arctic–midlatitude teleconnections show distinct changes. First, since the late 1990s, the relationship between December Bering Sea ice extent and January Siberian cold extremes has strengthened, supported by model experiments showing enhanced ridge–trough wave propagation into Eurasia. Second, targeted simulations demonstrate that November Arctic sea ice plays a critical role in modulating troposphere–stratosphere coupling, with a markedly weaker atmospheric response under late-autumn ice-free conditions. Third, large-ensemble simulations reveal that under strong CO₂ forcing, the historically robust “warmer Arctic–colder Eurasia” linkage weakens and becomes less coherent.

These results show that teleconnections in the New Arctic are increasingly season-dependent and state-dependent, with important implications for midlatitude climate variability and predictability.

How to cite: He, S., Fan, K., Zhao, J., Xu, X., and Jiang, J.: Teleconnections in the ‘new Arctic’, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17581, https://doi.org/10.5194/egusphere-egu26-17581, 2026.

EGU26-17796 | ECS | Posters on site | OS1.9

Tidal Forcing and Internal Wave Generation in the Arctic Ocean: High-Resolution FESOM Simulations 

Ekaterina Bagaeva, Friederike Pollmann, Qiang Wang, Patrick Scholz, and Sergey Danilov

Internal waves are a key driver of diapycnal mixing in the global ocean and play an essential role in setting the large-scale overturning circulation. In the Arctic Ocean, however, internal-wave-driven mixing is assumed to be weak due to strong stratification and the presence of sea ice, which limits wind forcing and surface wave activity. The scenario of ongoing sea-ice decline raises the possibility of enhanced internal wave activity and associated mixing, potentially increasing upward oceanic heat fluxes and further accelerating ice loss.

In this study, we investigate the role of tidal forcing as a source of internal waves in the Arctic Ocean using the ocean model FESOM. We perform simulations with tidal forcing at unprecedented horizontal resolution (around 1 km). The simulations are conducted for different seasons and sea-ice conditions to examine how variations in sea-ice modulate tidal currents and internal wave generation. By comparing simulations with and without tidal forcing, we assess the impact of tides on sea-ice dynamics, providing initial insight into coupling between tides, internal waves, and sea ice in the Arctic Ocean. The diagnosed internal tide generation will serve to force the internal wave model IDEMIX, which we will couple to FESOM to provide a consistent mixing parameterization for the simulation of the warming Arctic.

How to cite: Bagaeva, E., Pollmann, F., Wang, Q., Scholz, P., and Danilov, S.: Tidal Forcing and Internal Wave Generation in the Arctic Ocean: High-Resolution FESOM Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17796, https://doi.org/10.5194/egusphere-egu26-17796, 2026.

EGU26-17934 | Orals | OS1.9

AWI-ESM3 high resolution model contribution to CMIP7: First results of the model response in the Arctic regions during the historical period 

Nadine Wieters, Jan Streffing, Laszlo Hunor Hajdu, Helge F. Goessling, and Thomas Jung

Earth system modelling is an important instrument to investigate climate change in an integrated way, taking into account the interactions between the different compartments of the Earth system. It is also an important tool to perform climate projections for different climate scenarios in order to take appropriate mitigation and adaptation measures. Such climate simulations are coordinated internationally as part of the World Climate Research Programme’s (WCRP) Coupled Model Intercomparison Project Phase 7 (CMIP7).
The Alfred Wegener Institute (AWI) will participate in the CMIP7 project with the Earth system model AWI-ESM3. This is being done as part of the German contribution to the Coupled Model Intercomparison Project (CAP7).
One focus of our work is the impact of anthropogenic aerosol forcing during the historical CMIP7 period. Earlier versions of the AWI climate model setup used a fixed aerosol climatology and thus clearly overestimated the temperature increase for the historical period due to the lack of changing direct and indirect aerosol effects. The implementation of transient aerosols brings the simulated historical period closer to observed trends.
In this presentation we will show first results of the CMIP7 historical experiment performed by the AWI-ESM3 high resolution model including the impact of transient aerosol forcing. We will discuss the results with respect to the Arctic regions and the comparison to observations and climate performance indices.

How to cite: Wieters, N., Streffing, J., Hajdu, L. H., Goessling, H. F., and Jung, T.: AWI-ESM3 high resolution model contribution to CMIP7: First results of the model response in the Arctic regions during the historical period, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17934, https://doi.org/10.5194/egusphere-egu26-17934, 2026.

EGU26-18611 | Orals | OS1.9

Exploring density flux variability in the Nordic Seas through new satellite products: Insights from ESA’s Polar Science Cluster ARCTIC-FLOW project 

Veronica Gonzalez Gambau, Manuel Arias, Joan Bergas-Ques, Agnieszka Beszczynska-Möller, Carolina Gabarro, Aina García-Espriu, Ilona Goszczko, Michael Karcher, Nanna B. Karlsson, Frank Kauker, Estrella Olmedo, Aqeel Piracha, Arnau Ruiz-Sebastián, Roberto Sabia, Ana Sagués, Antonio Turiel, Marta Umbert, Artemis Vrettou, and Martin Wearing

The Atlantic Meridional Overturning Circulation (AMOC) plays a central role in the climate system by transporting and redistributing heat to depth, thereby regulating the effective heat capacity of the ocean under global warming. Observations and projections indicate a potential decline of the AMOC in response to climate change, with far-reaching climate consequences. The Nordic Seas are a key region for the overturning circulation, as dense water formation north of the Greenland–Scotland Ridge feeds the lower limb of the AMOC.

Within this context, the ARCTIC-FLOW project aims to improve our understanding of water mass transformation and overturning processes in the Nordic Seas. The project focuses on identifying the main regions of surface water transformation, quantifying water mass transformation rates, characterizing the temporal and spatial scales of dense water formation, and assessing the impact of extreme freshening events across different subregions of the Nordic Seas.

To support these objectives, we have developed a novel 11-year satellite-based time series of freshwater and density fluxes for the Arctic and sub-Arctic regions. This dataset is derived from the combination of satellite sea surface salinity, sea surface temperature, and surface velocity fields, together with information on mixed layer depth. The satellite products are evaluated and complemented using an extensive set of in situ observations and results from numerical model experiments.

In this contribution, we will present preliminary results on the variability of the newly developed satellite-derived density flux product, highlighting its relevance for studying variability of water-mass transformation processes in the Nordic Seas.

 

How to cite: Gonzalez Gambau, V., Arias, M., Bergas-Ques, J., Beszczynska-Möller, A., Gabarro, C., García-Espriu, A., Goszczko, I., Karcher, M., Karlsson, N. B., Kauker, F., Olmedo, E., Piracha, A., Ruiz-Sebastián, A., Sabia, R., Sagués, A., Turiel, A., Umbert, M., Vrettou, A., and Wearing, M.: Exploring density flux variability in the Nordic Seas through new satellite products: Insights from ESA’s Polar Science Cluster ARCTIC-FLOW project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18611, https://doi.org/10.5194/egusphere-egu26-18611, 2026.

EGU26-19573 | ECS | Orals | OS1.9

Changes in water mass composition and circulation in the central Arctic Ocean between 2011 and 2021 inferred from tracer observations 

Anne-Marie Wefing, Annabel Payne, Marcel Scheiwiller, Christof Vockenhuber, Marcus Christl, Toste Tanhua, and Núria Casacuberta

The Arctic Ocean is changing rapidly, and Atlantic Water circulation plays a key role in the warming, sea-ice decline, and ecosystem changes observed in the Arctic. Still, we have limited understanding of the pathways and circulation times of Atlantic-derived water both at surface and mid-depth layers in the Arctic Ocean, and their evolution over time.

Here, we present the water mass composition and circulation in the central Arctic Ocean in 2021 and assess temporal changes thereof between 2011 and 2021 by using the long-lived anthropogenic radionuclides I-129 and U-236 in the Transit Time Distribution model. Key findings for 2021 include a decline in surface radionuclide concentrations between the Amundsen and Makarov Basins, pointing to substantial fractions of Pacific Water reaching the Lomonosov Ridge from the Amerasian side. Similar radionuclide concentrations in halocline waters on both sides of the Lomonosov Ridge suggest a common formation region of these waters with a clear Atlantic Water signal. North of Greenland, a mixture of waters from the Canada and Amundsen Basins is observed at both surface and mid-depth. Between 2011 and 2021, we observe a shift of the Atlantic-Pacific Water front from the Makarov Basin towards the Lomonosov Ridge and an increase in circulation times in the mid-depth Atlantic layer. Overall, our findings provide a baseline of the circulation of Atlantic-derived waters in 2021 and provide evidence of circulation changes both in the surface and intermediate waters between 2011 and 2021.

How to cite: Wefing, A.-M., Payne, A., Scheiwiller, M., Vockenhuber, C., Christl, M., Tanhua, T., and Casacuberta, N.: Changes in water mass composition and circulation in the central Arctic Ocean between 2011 and 2021 inferred from tracer observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19573, https://doi.org/10.5194/egusphere-egu26-19573, 2026.

EGU26-21848 | ECS | Orals | OS1.9

Constraining Mercury Sources to the Arctic Ocean Using Mercury Stable Isotopes 

Alina Kleindienst, Ilaria Barale, Julie Lattaud, Stephen G. Kohler, Lars-Eric Heimbürger-Boavida, Oleg S. Pokrovsky, Jeroen Sonke, and Sofi Jonsson

Mercury (Hg) concentrations in Arctic biota are elevated relative to lower latitudes, posing an increased risk of adverse health effects for Arctic populations that rely on them as an important food source. Hg readily cycles through different environmental compartments such as air–soil–river before reaching sea waters where it becomes available for methylation to methylmercury and is readily taken up and magnified in the marine food web.

Warming climate is expected to further enhance air-soil-river exchange, increase river discharge, mobilize additional Hg loads from thawing permafrost, erosion melting glaciers and sea ice. A recent Arctic Ocean (AO) Hg mass budget indicates that Hg inputs exceed outputs, indicating either a missing sink or an imbalance due to ongoing changes. 

We determined Hg stable isotope endmember signatures of Hg sources, including western Siberian organic-rich permafrost and mineral soils, and compile those with available literature data on endmembers. Central AO surface seawater samples were collected under trace metal clean conditions in Summer 2025 aboard RV ODEN and zooplankton samples in Summer 2015 aboard RV Polarstern. Solid samples were pre-concentrated using a double tube furnace set-up, while 40 L of sea water were pre-concentrated using a two-step purge and trap method. Hg stable isotopic composition was measured via online cold-vapor generation multicollector ICP-MS analysis.

We use the new Hg stable isotopes measurements together with available literature data to better constrain the Arctic Hg cycle by disentangling the relative importance of different Hg sources to AO surface waters, the entry point of Hg into the marine food web.

How to cite: Kleindienst, A., Barale, I., Lattaud, J., Kohler, S. G., Heimbürger-Boavida, L.-E., Pokrovsky, O. S., Sonke, J., and Jonsson, S.: Constraining Mercury Sources to the Arctic Ocean Using Mercury Stable Isotopes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21848, https://doi.org/10.5194/egusphere-egu26-21848, 2026.

EGU26-22061 | Orals | OS1.9

Decadal coherence of Arctic thermohaline staircases 

Erica Rosenblum, Mikhail Schee, Jonathan Lilly, and Nicolas Grisouard

Thermohaline staircase layers have been consistently observed in the Arctic Ocean for over 50 years. Previous studies demonstrate that these structures exhibit large-scale spatial coherence.  However, on time scales beyond a few years, both the coherence and evolution of the layers are unknown. Using Ice-Tethered Profiler data from 2005--2022 in the Beaufort Gyre Region, we track staircase layers across time and space with an unsupervised clustering method. Individual layers are found to be coherent across the entire 17-year time period, with properties that appear to evolve on 40--50 year timescales or longer. This establishes, for the first time, the decadal-scale coherence of thermohaline staircases in the Arctic Ocean. Moreover, we find that the observed changes are not consistent with the staircase being in a state of equilibrium, but rather support the hypothesis that it is decaying slowly from an initial or on-going perturbation.

How to cite: Rosenblum, E., Schee, M., Lilly, J., and Grisouard, N.: Decadal coherence of Arctic thermohaline staircases, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22061, https://doi.org/10.5194/egusphere-egu26-22061, 2026.

EGU26-22753 | Orals | OS1.9

Observations of ducting of acoustic energy in the Fram Strait. 

Giacomo Giorli, Silvia Falchetti, Aniello Russo, and Gaultier Real

Arctic areas like the Beaufort Sea are commonly characterized by the formation of sub-surface acoustic ducts. Conversely, the eastern Arctic is known for its upward refracting propagation environment, which creates surface ducts. Using moored passive acoustic recorders in the Fram Strait in the eastern Arctic Ocean, we measured the average distribution of sound energy in the water column. The moorings were deployed by the CMRE Environmental Knowledge and Operational Effectiveness program and instrumented with several oceanographic sensors and acoustic recorders. Even though some acoustic recorders failed to record for the entire experiment, we characterized the vertical distribution of the ambient noise field. We measured the formation of temporary sound energy duct-type areas in the thermocline. Using Copernicus Marine service data, we investigated the effects of the sea ice concentrations, sea ice drift and distance to the sea ice edge on the vertical distribution of ambient noise. The distance from the ice edge had a negative correlation with sounds levels, while ice drift and concentration were not correlated to the overall sound levels. Simultaneous sound speed measurements revealed the presence of potential sound channels. We investigated the possible origin of the sound energy, and the formation of potential sub-surface ducts, applying range-dependent sound propagation modelling coupled with high-resolution output of the double nested CMRE’s Pan-Arctic ocean-sea ice model.

How to cite: Giorli, G., Falchetti, S., Russo, A., and Real, G.: Observations of ducting of acoustic energy in the Fram Strait., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22753, https://doi.org/10.5194/egusphere-egu26-22753, 2026.

EGU26-22763 | Orals | OS1.9

Multi-domain environmental sensing for underwater acoustics in the Arctic marginal ice zone. 

Gaultier Real, Giuliana Pennucci, F. Hunter Akins, and Tommaso Fabbri

Recent and rapid environmental changes in the Arctic Ocean lead scientists to re-evaluate the way they operate in this area. NATO STO Centre for Maritime Research and Experimentation (CMRE) leads the Nordic Recognised Environmental Picture (NREP) trial series in order to understand how a better characterization of the Arctic environment is possible and how it can help to build more accurate underwater acoustic modelling capabilities. NREP25 was conducted in the Greenland Sea from July 16th to July 27th 2025. On-board NATO Research Vessel (NRV) Alliance, underwater acoustic propagation experiments were performed in various Arctic environments (packed ice, marginal ice, open waters, brash ice), deploying in-house built receivers alongside other innovative solutions. NRV Alliance acted as the acoustic source, transmitting pre-defined sequences of known waveforms that will be used for probing the Arctic environment, in particular the interactions of sound waves with the space and time-dependent ice cover. The latter was estimated using a combination of remote sensing capabilities. First, a new prototype of ship-borne X-band RADAR provided a continuous estimation of the positions of the ice floes. Second, remote sensing imagery from diverse satellites (Sentinel, COSMO-SkyMed, SWOT and RADARSAT) provided high-resolution images of the sea ice cover, obtained from SAR processing, several times a day. NRV Alliance also served as a “floating ground control” for drone activities. Namely, high resolution photogrammetry and point-cloud LiDAR data were obtained from aerial drone surveys. 

Oceanographic characterization was carried out through extensive CTD casts, as well as glider missions (with acoustic payloads as well). This characterization was used to design experimental configurations that were more likely to generate interactions of acoustic paths with the sea ice at the surface.

In addition, CMRE conducted specific characterization of the water ice interface by ROV inspection (with video, acoustic camera and altimetry data), and also ice coring (to be analysed at the centre).

An overall description of the experiment is presented, as well as an analysis of the data collected focusing on the contribution of remote sensing to the understanding of the underwater acoustic observations.

How to cite: Real, G., Pennucci, G., Akins, F. H., and Fabbri, T.: Multi-domain environmental sensing for underwater acoustics in the Arctic marginal ice zone., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22763, https://doi.org/10.5194/egusphere-egu26-22763, 2026.

EGU26-22970 | Posters on site | OS1.9

The CASCADES Expedition: multidisciplinary observations of a rapidly changing Arctic 

Bastien Ruols, Jean-Éric Tremblay, Samuel Jaccard, and Dany Dumont

 The Arctic, spanning over eight sovereign countries and the Arctic Ocean, is warming three tofour times faster than the global average, driving profound transformations of the cryosphereand ocean systems. It harbours four critical climate tipping points: the accelerated melt of theGreenland Ice Sheet, the thawing of boreal permafrost, the collapse of winter Arctic sea ice,and the weakening of the Labrador–Irminger Seas convection. These processes are tightlyinterconnected and play a key role in regulating the global climate, yet their combined impactsremain insufficiently constrained by observations.Within this context, the CASCADES Expedition is an international and interdisciplinary polarprogramme designed to investigate the coupled interactions between glaciers, sea ice, and theocean around Baffin Bay and Northwest Greenland. CASCADES is coordinated by the InstitutNordique du Québec, the Swiss Polar Institute, and the French Polar Institute, in collaborationwith Greenlandic institutions. It brings together more than 50 Canadian, French, Greenlandic,and Swiss researchers around 16 scientific projects from 13 research institutions.CASCADES will be conducted aboard the Canadian research icebreaker CCGS Amundsen andis structured into two complementary legs in 2026, aligned with critical seasonal phases of theArctic system. A first leg during the summer targets peak glacier melt and freshwater input,while a second leg during autumn focuses on the transition toward sea-ice freeze-up. This dual-season strategy enables the investigation of how physical, chemical, and biological processesevolve from melt to freeze-up, and how these transitions affect carbon cycling, productivity,and ecosystem structure.By providing coordinated, multidisciplinary observations across key Arctic seasons,CASCADES aims to improve understanding of cryosphere–ocean–ecosystem coupling and itsimplications for the North Atlantic and the global climate system. Beyond its core scientificobjectives, the expedition serves as a platform for international collaboration, sciencediplomacy, education, and engagement with Arctic communities, contributing to sharedobservation efforts and to the anticipation of climate-driven changes in polar oceans and beyond.

How to cite: Ruols, B., Tremblay, J.-É., Jaccard, S., and Dumont, D.: The CASCADES Expedition: multidisciplinary observations of a rapidly changing Arctic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22970, https://doi.org/10.5194/egusphere-egu26-22970, 2026.

EGU26-506 | ECS | Orals | OS1.6

Climate state dependent sedimentation dynamics in the southern Scotia Sea during the last four glacial cycles 

Moritz Hallmaier, Marcus Gutjahr, Sidney R. Hemming, Jörg Lippold, Michael E. Weber, and Anton Eisenhauer

The Southern Ocean (SO) is of major importance in shaping climate transitions due to its substantial potential in storing carbon in the deep ocean and its release to the atmosphere most dominantly during glacial terminations. Through wind driven upwelling of deep waters and high latitude deep water formation, the SO acts as a gateway between the surface ocean and its interior. With the Antarctic Circumpolar Current (ACC), the world’s largest current system, the SO connects all three major basins of the global ocean and therefore integrates and responds to climate signals across the globe. Additionally, the SO exerts a major influence on the Antarctic Ice Sheet and partly controls its mass balance.

The evolution of deep-water formation and export, as well as its interplay with the ACC and the Antarctic Ice Sheet are important factors that are still poorly constrained. We present a largely isotope geochemical based high-resolution multi-proxy reconstruction of IODP Site U1537 to examine these interplays in the southern Scotia Sea. The Scotia Sea is a key area in the SO, where newly formed well ventilated Weddell Sea Deep Water (WSDW) is admixed into and entrained underneath the ACC.

Sedimentation in this area is mainly modulated by the strong ocean currents, as seen by extremely high sediment focusing throughout. Detrital neodymium (Nd) as well as authigenic and detrital lead (Pb) isotope compositions in Southern Ocean sediments provide insights into sediment sources, which can be clearly identified due to the distinct crustal ages of East and West Antarctica and its surrounding areas. Sediments at Site U1537 are dominantly sourced from the Antarctic Peninsula and the Weddell Sea region. The sediment provenance investigations are additionally complemented by K’-Ar analyses on the <63 µm fractions of the sediment samples, providing average age information. All of our obtained isotopic records reveal substantial variations during glacial-interglacial transitions.

Site U1537 provides evidence for low bottom water oxygenation (derived from authigenic uranium) and likely no WSDW export into the Scotia Sea during the Last Glacial Maximum. The data further suggests early deglacial pulses of WSDW export. We advocate that these pulses might be a considerable contributor to the reestablishment of interglacial-type deep ocean ventilation and AMOC conditions. A substantial increase in current-shelf interaction along the Antarctic margin in the Pacific sector is seen during MIS5e. Taken together, our multi-proxy approach highlights the complex sedimentation regime in the Scotia Sea and provides new paleoceanographic insights towards the circulation and frontal dynamics as a function of climatic boundary conditions at submillennial-scale resolution.

How to cite: Hallmaier, M., Gutjahr, M., Hemming, S. R., Lippold, J., Weber, M. E., and Eisenhauer, A.: Climate state dependent sedimentation dynamics in the southern Scotia Sea during the last four glacial cycles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-506, https://doi.org/10.5194/egusphere-egu26-506, 2026.

Phaeophyta (i.e., brown seaweeds) are significant primary producers in high-latitude environments, serving as a key nutritional source to fauna and carbon sink. Despite being the dominant biomass source in polar regions, they have largely been overlooked in carbon assessments, trophic ecology, and biogeochemical studies. Our understanding of how these ecosystems will respond to climate change is limited, based on a handful of studies that are primarily Arctic focussed. Stable carbon (δ13C) and nitrogen (δ15N) isotope analysis of macroalgae has often been used as a tool to assess nutrient sources, energy transfer and photosynthetic mechanism but has rarely been applied to polar macroalgae. The rapid environmental change in both poles has the potential to shift the isotopic baseline. Our current understanding is poor, to our knowledge only 28 studies have published biogeochemical assessments of Antarctic macroalgae, half of which are from the South Shetland Islands in the northern West Antarctic Peninsula. Yet biogeochemical data can provide a wealth of information regarding nutrient source changes, light dynamics, productivity and nutritional quality. Larger species, such as Himantothallus grandifolius (Antarctic) or Saccharina latissima (Arctic) can provide seasonal or even multi-annual data through incremental stable isotope analysis along macroalgal blades. Changing productivity rates can be tracked through δ13C values, fluctuating due to sea ice break out, carbon demand and growth requirements. Over 20 specimens of H. grandifolius and Arctic kelps have been collected over several field trips to the Antarctic Peninsula, East Greenland coastline and Svalbard for δ13C and δ15N analysis; forming the largest biogeochemical dataset for polar macroalgae to date. Large variations > 15 ‰ were recorded for the Antarctic species H. grandifolius from a single organism, a significant variation when considering trophic level shifts are on a scale of ~ 3–5 ‰. Cyclical trends in productivity were also identified in several specimens with wider implications for shifting isotopic baselines of primary producers in response to environmental change on seasonal and multi-year time scales. Strong seasonal responses in δ13C are linked to sea ice and fluctuating light conditions with increased run off through glacial melting. Nitrogen was found to vary between sub-tidal and inter-tidal species, as well as incrementally along blades of larger species. New nitrogen sources may be introduced to remote polar regions as increased tourism increases the risk of wastewater and pollutant inputs to these fragile ecosystems. Macroalgae could become an ideal tracer in coastal environments where nutrient sources can be assessed at varying time scales.

Our incremental approach provides high resolution isotopic data with the capacity to generate seasonal to multi-year records from an understudied ecosystem. Polar environments are set to change in unprecedented ways, the shifting isotopic baseline has repercussions for the wider food web, ecosystem structure and functioning that macroalgae play a key role in.

How to cite: Alldred, F. and Gröcke, D.: Stable isotope analysis of polar seaweeds: Assessing productivity and response to environmental change on seasonal and multi-annual time scales, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-722, https://doi.org/10.5194/egusphere-egu26-722, 2026.

EGU26-1071 | ECS | Orals | OS1.6

Hydrothermal Plumes in the Arctic Ocean -The Aurora Site at Gakkel Ridge 

Jonathan Mette, Maren Walter, Jürgen Sültenfuß, and Christian Mertens and the R/V Polarstern PS137 Science Team

Hydrothermal venting along mid-oceanic ridges alters deep ocean water masses around the globe. These vent systems supply geothermal heat and various biogeochemical properties to water masses close to the bottom. In the Arctic, the influence of hydrothermal venting is largely unknown, and whether it should be considered in relation to other processes that modify the highly isolated deep water masses.

We present new results from the expedition PS 137 on water masses and the flux associated with the Aurora Vent Site at the Gakkel Ridge, 82.9° N, the only system in the Arctic Ocean to have been visited twice. Utilising CTD observations including physical and biogeochemical data, we assess the dimensions of the hydrothermal plume and estimate the heat flux. A spatially restricted plume core with a horizontal extent of less than 1000 m but a large rise height of 1200 m above the seafloor results in an estimated heat flux of approximately 180 MW.

A comparison with the observations made in 2014 reveals that the plume exhibits a comparable height, suggesting a constant heat flux over the period. Furthermore, the combined helium isotope measurements indicate that water masses on a larger scale at the Gakkel Ridge are also influenced by hydrothermal systems.

How to cite: Mette, J., Walter, M., Sültenfuß, J., and Mertens, C. and the R/V Polarstern PS137 Science Team: Hydrothermal Plumes in the Arctic Ocean -The Aurora Site at Gakkel Ridge, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1071, https://doi.org/10.5194/egusphere-egu26-1071, 2026.

Dissolved oxygen is a key indicator of ocean health and is being altered by climate-driven warming. The Arctic–subarctic system is warming at an exceptional pace due to Arctic amplification, but how this rapid warming translates into basin-wide oxygen change is still not well constrained. Using observations of Atlantic Water (AW) pathways, we find that the Atlantic inflow exerts a leading control on recent deoxygenation in the Arctic Ocean. Oxygen declines are detected in the upper eastern Arctic and in the intermediate layers of the western Arctic at rates of −0.41 ± 0.17 to −0.47 ± 0.07 μmol kg−1 yr−1, approximately six times the global mean. We identify amplified warming in Arctic gateway regions as the dominant driver, primarily through a strong reduction in oxygen solubility. The resulting low-oxygen signal is then propagated into the interior Arctic by rapid subduction and circulation of AW, extending the impact to deeper layers and increasing risks to Arctic marine ecosystems. These results emphasize that warming Atlantic inflow is central to shaping Arctic oxygen dynamics; continued temperature rise is therefore expected to sustain and potentially strengthen ongoing deoxygenation, calling for heightened attention and broader monitoring across the Arctic.

How to cite: Wu, Y.: Arctic amplification–driven warming of Atlantic inflow intensifies oxygen loss across the Arctic Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2655, https://doi.org/10.5194/egusphere-egu26-2655, 2026.

EGU26-6434 | ECS | Orals | OS1.6

Growing Influence of Indian Ocean Waters in the South Atlantic Intermediate Layer over the last 30 years 

Zhetao Tan, Elaine McDonagh, Sabrina Speich, Cristian Florindo Lopez, Xabier Davila Rodriguez, and Emil Jeansson

Global climate change is concurrently and profoundly altering the ocean’s physical and biogeochemical environment. The intermediate water in the South Atlantic and Indian Oceans, which together constitute a critical component of the upper limb of the Atlantic Meridional Overturning Circulation (AMOC), lies at the heart of these changes. The intermediate layer of the South Atlantic is ventilated by two primary sources: relatively fresher and younger waters (characterised by low Apparent Oxygen Utilization, AOU) originating from the Pacific Ocean, and saltier and older waters advected from the Indian Ocean via the Agulhas System. However, the extent to which the intrusion of saline, older Indian Ocean waters via the Agulhas System modulates the stability of the AMOC’s upper limb remains poorly understood. Specifically, the temporal variability and long-term contribution of the Indian Ocean waters to the South Atlantic intermediate layer remains a knowledge gap.

Here, we focus on observational evidence of and investigate the underlying mechanisms driving the influence of Indian Ocean intermediate waters on the Atlantic Ocean in a warming climate. We examine AOU-salinity covariability across decadal to multi-decadal time scales within South Atlantic intermediate water. This analysis integrates high-quality observational databases of temperature, salinity, dissolved oxygen, and water age, as well as repeat hydrographic sections, allowing us to link their observed variability to changes in circulation and mixing, while considering oxygen disequilibrium effects and the influence of the biological carbon pump in changing AOU.

We find an increasing influence of Indian Ocean water in the South Atlantic at the intermediate layer over the past 30 years. The most strongly impacted regions are identified. In addition, we quantify the impact of Indian Ocean influence on the South Atlantic and show that this signal has become progressively detectable over the past 30 years, but has not yet exceeded the level of internal variability, indicating an ongoing ‘Indianization’ of the South Atlantic intermediate layer. We identify the underlying mechanisms related to the increasingly positive phase of the Southern Annular Mode (SAM) and an associated multidecadal increase in Agulhas leakage. Finally, we will discuss the potential implications of this phenomenon for the long-term stability of the AMOC.

How to cite: Tan, Z., McDonagh, E., Speich, S., Florindo Lopez, C., Davila Rodriguez, X., and Jeansson, E.: Growing Influence of Indian Ocean Waters in the South Atlantic Intermediate Layer over the last 30 years, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6434, https://doi.org/10.5194/egusphere-egu26-6434, 2026.

EGU26-6726 | ECS | Orals | OS1.6

Improving polar ocean temperature reconstructions with crust-lamellae specific Mg/Ca-temperature calibrations and improved understanding of its non-thermal forcers 

Adele Westgård, Mohamed M. Ezat, Freya E. Sykes, Julie Meilland, Thomas B. Chalk, J. Andy Milton, Melissa Chierici, Jochen Knies, and Gavin L. Foster

Reconstructing past ocean-cryosphere interactions can provide crucial insight to the ongoing rapid climate change in the polar regions and beyond. However, there are large uncertainties in existing proxies commonly used in downcore reconstructions, including a lack of low-temperature (<9°C) culture-based Mg/Ca-temperature calibrations for planktic foraminifera. In the polar oceans the foraminiferal assemblage is not diverse and commonly dominated by Neogloboquadrina pachyderma, yet there is limited understanding of non-thermal influences on this proxy in this species. N. Pachyderma also precipitates a thick low-Mg/Ca crust over its inner higher Mg/Ca lamellar calcite, that contributes to uncertainties and inaccuracies in high-latitude palaeotemperature reconstructions.

To address this, we cultured N. pachyderma across a 2 to 9°C temperature range, at a range of salinities (29.8–36.6), and carbonate chemistry conditions with both co-varying and decoupled pH (7.65–8.4) and [CO32-] (64–243 µmol/kg) and analysed their trace element composition using Laser Ablation Inductively Coupled Plasma Mass Spectrometry.

We present a new method that distinguishes the crust and lamellar calcite using trace element profiles from both cultured and fossil shells. This allowed us to show distinct geochemical signals in the crust and lamellar calcite of laboratory-grown N. pachyderma, including lower Mg/Ca, Na/Ca, and B/Ca in the crust compared to the lamellar calcite. We present new Mg/Ca-relationships, with independent calibrations for the crust and lamellar calcite. The temperature calibrations extend the lower range of culture-based Mg/Ca-calibrations down to 2°C. Furthermore, we show significant and opposing pH and [CO32-] influences on Mg/Ca when these variables are decoupled and no statistically significant influence of salinity on Mg/Ca. Crust and lamellar calcite element/Ca are found to have different sensitivities to changing environmental conditions. Our results also show that environmental conditions control the crust-lamellar proportions and shell thickness which has implications for both downcore reconstructions and ongoing ocean acidification and warming.

Overall, our findings suggests that the crust and lamellar calcite precipitate via contrasting biomineralisation strategies and/or varying precipitation rates, leading to distinct geochemical compositions and different sensitivities to changing environmental conditions. We propose that distinguishing the two components and applying Mg/Ca-environmental relationships with separate calibrations for the crust and lamellar calcite will substantially reduce uncertainties in high-latitude palaeoceanographic reconstructions. We are now in the process of applying these methods and relationships to Quaternary sediment records from the central Arctic Ocean and the Nordic Seas.

How to cite: Westgård, A., Ezat, M. M., Sykes, F. E., Meilland, J., Chalk, T. B., Milton, J. A., Chierici, M., Knies, J., and Foster, G. L.: Improving polar ocean temperature reconstructions with crust-lamellae specific Mg/Ca-temperature calibrations and improved understanding of its non-thermal forcers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6726, https://doi.org/10.5194/egusphere-egu26-6726, 2026.

EGU26-8075 | Posters on site | OS1.6

Antarctic krill connectivity: a Lagrangian modeling framework to understand Southern Ocean population dynamics 

Olivier Gourgue, Léo Barbut, Antoine Barthélémy, Valérie Dulière, Thierry Fichefet, Emmanuel Hanert, Geneviève Lacroix, François Massonnet, Benjamin Richaud, Isa Schön, Zephyr Sylvester, and Anton Van de Putte

Antarctic krill populations exhibit substantial interannual fluctuations with highly variable success in the survival of larvae to the juvenile stage. Understanding connectivity between spawning hotspots and the areas where larvae successfully develop into juvenile populations is essential for predicting population dynamics and informing fishery management, yet the drivers of krill connectivity variability across the Southern Ocean remain poorly quantified.

This project uses Lagrangian particle tracking simulations to investigate krill larval connectivity patterns over 30 years (1993-present) based on high-resolution ocean circulation model outputs. We release over a billion virtual larvae throughout the spawning season across known spawning grounds and track their drift to quantify: (1) the variability of natural connectivity  among populations, (2) how spawning timing influences dispersal success, and (3) which large-scale climate patterns (SAM, ENSO, ACC variability) drive strong versus weak connectivity years.

Network analysis identifies critical source populations that supply multiple recruitment areas and vulnerable sink populations dependent on external larval input. This connectivity baseline is essential for distinguishing natural fluctuations from climate-driven changes in future projections.

Results will inform the Commission for the Conservation of Antarctic Marine Living Resources (CCAMLR) by revealing which populations require protection and identifying critical hubs that sustain networks of connected krill populations. The Lagrangian model framework and open-source outputs will provide a foundation for subsequent climate change projections examining how changes in Southern Ocean circulation may alter connectivity patterns by 2050-2100.

How to cite: Gourgue, O., Barbut, L., Barthélémy, A., Dulière, V., Fichefet, T., Hanert, E., Lacroix, G., Massonnet, F., Richaud, B., Schön, I., Sylvester, Z., and Van de Putte, A.: Antarctic krill connectivity: a Lagrangian modeling framework to understand Southern Ocean population dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8075, https://doi.org/10.5194/egusphere-egu26-8075, 2026.

EGU26-8271 | ECS | Orals | OS1.6

Evidence for Pliocene North Pacific Deep Water Formation and Its Paleoproductivity Imprints 

Yongzhi Chu, Ruiling Zhang, Xiaohu Li, Ruifang Xie, Weiqi Yao, and Antao Xu

Deep-water formation plays a crucial role in global climate, yet it is absent in the modern North Pacific. However, the existence of North Pacific Deep Water (NPDW) formation during the Pliocene and its impact on the marine carbon cycle remain controversial. Here, we present high-resolution sedimentary records of authigenic neodymium isotope composition(εNd), barite accumulation rates (BAR), and barite barium (Ba) isotope compositions (δ138Babarite) from ODP Site 882 in the subarctic Northwest Pacific.

Our results reveal pronounced shifts in εNd and Ba-proxy records synchronous with the intensification of Northern Hemisphere Glaciation. Specifically, across the ~2.73 Ma interval, seawater εNd values decrease from +0.2 to -1.4, marking a shift from northern-sourced NPDW to southern-sourced Pacific Deep Water (PDW). This circulation collapse was accompanied by elevated BAR and δ138Babarite values, indicating a transient peak in export production. Intriguingly, this productivity pulse is decoupled from biogenic opal accumulation, which declines during the same interval. We propose that the cessation of NPDW formation allowed the upwelling of nutrient-rich PDW. This process fueled a transient increase in export production but partly drove the ecosystem from a silicate-replete to a silicate-limited regime, or reduced nutrient burial efficiency.

In contrast to the dynamic Late Pliocene, our new data from the Early Pliocene (~4.3–3.6 Ma) show relatively stable εNd and Ba-proxy records. These findings challenge previous hypotheses of an Early Pliocene circulation transition derived from Japan Sea records, suggesting that open ocean circulation in the subarctic Pacific remained stable prior to the onset of major glaciations. Our study highlights the critical role of physical circulation thresholds in regulating the efficiency of the biological carbon pump and nutrient inventory in the North Pacific.

How to cite: Chu, Y., Zhang, R., Li, X., Xie, R., Yao, W., and Xu, A.: Evidence for Pliocene North Pacific Deep Water Formation and Its Paleoproductivity Imprints, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8271, https://doi.org/10.5194/egusphere-egu26-8271, 2026.

EGU26-8433 | ECS | Posters on site | OS1.6

Changes in the Southern Ocean over the last two decades from Argo float measurements 

Ana Amaral Wasielesky, Milena Menna, Elena Mauri, Angelo Rubino, Riccardo Martellucci, and Melissa Bowen

The Southern Ocean (SO) plays a crucial role in connecting all the world's oceans through the Antarctic Circumpolar Current (ACC). Global ocean circulation is also affected by processes in the Southern Ocean that change the density and subduction rate of water. Argo has provided consistent and basin-wide coverage of this region over the past two decades, enabling analyses not possible with the sparse and episodic ship-based observations available earlier. This study uses the Argo float  dataset collected between 2004 and 2025  along the ACC. The data was gridded and processed using the pseudoeulerian approach; the full dataset and decadal differences were obtained for 18 sections of the SO. We will present the spatial variability of water masses in the Southern Ocean, highlighting their decadal and interannual variability and the associated large-scale spatial gradients relevant to Southern Ocean dynamics. The use of Argo float observations provides unprecedented details for examining the spatial and temporal evolution of density patterns resulting from salinity and temperature changes, with important implications for global ocean circulation and climate.

How to cite: Amaral Wasielesky, A., Menna, M., Mauri, E., Rubino, A., Martellucci, R., and Bowen, M.: Changes in the Southern Ocean over the last two decades from Argo float measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8433, https://doi.org/10.5194/egusphere-egu26-8433, 2026.

EGU26-10619 | ECS | Posters on site | OS1.6

Neodymium Cycling and Water Mass Structure in the Indian Sector of the Southern Ocean 

Manuel Ehnis, Marcus Gutjahr, David Menzel, Huang Huang, Layla Creac'h, Annika Oetjens, Ole Rieke, Laura Herraiz Borreguero, Markus Janout, Jörg Rickli, Martin Frank, Sandra Tippenhauer, and Jörg Lippold

The Southern Ocean plays a central role in the global climate system by regulating large-scale circulation, facilitating interbasin exchange, absorbing large amounts of anthropogenic heat and carbon and influencing Antarctic Ice Sheet stability. Yet, observational data, including rare earth element measurements such as neodymium (Nd) isotopes and samarium (Sm), have so far remained sparse in the Indian sector and along the East Antarctic continental margin, thereby limiting our understanding of circulation, water mass transformation, and sediment-ocean interactions in a changing climate.

Water masses in the Southern Ocean are traditionally characterized using hydrographic parameters (e.g., potential temperature, salinity, neutral density). During physico-chemical weathering along the East Antarctic margin, old continental crust supplies a distinctly unradiogenic neodymium isotope signature (low εNd) to regional shelf waters that interact with more radiogenic Antarctic Circumpolar Current waters (higher εNd) further north. This isotopic difference makes neodymium isotopes an especially powerful tracer of regional circulation and mixing along the East Antarctic continental margin. We present the first high-resolution dataset of dissolved εNd, together with Nd and Sm concentrations, from the Indian sector of the Southern Ocean. Gridded water column samples in conjunction with bottom water samples extracted from multicorer sediment supernatants, collected during expedition EASI-2 onboard RV Polarstern (Dec 2023–Feb 2024), provide a meridional transect from the Denman Glacier front (~66°S) to ~45°S along 100°E. Combined with hydrographic observations, this dataset provides a detailed framework for examining water mass structure, mixing, and regional boundary fluxes along the transect.

Away from direct Antarctic continental influences, the εNd distributions show largely conservative behavior in intermediate to deep waters and allow clear identification of major Southern Ocean water masses. A striking feature is the persistence of a remnant North Atlantic Deep Water εNd signal within lower Circumpolar Deep Water, highlighting long-range interbasin connectivity. Near the Denman Glacier, warm and radiogenic modified Circumpolar Deep Water (mCDW) intrudes onto the continental shelf, evident in both physical properties and εNd signatures below ~400 meters water depth. As seen in earlier studies, a pronounced mCDW tongue was observed to reach close to the Denman Glacier front, with associated high basal melt rates evident from potential temperature and salinity in sampled local East Antarctic shelf waters.

Nd and Sm concentrations increase linearly with depth north of the Polar Front, but exhibit substantial enrichment south of the front, reflecting deep-water upwelling, biogenic scavenging, and a latitudinally gradual boundary exchange. Pronounced variations in εNd and rare earth element concentrations in bottom waters point to substantial benthic additions in the southern reaches of the transect driven by weathering inputs from ambient terrigenous sediments, whereas particle-related scavenging appears to dominate offshore.

This study closes a critical observational gap in the Indian sector of the Southern Ocean and provides new constraints on the present-day circulation, water mass structure, and the influence of Antarctic crustal and benthic Nd additions, while demonstrating the value of εNd as a tracer in modern and paleoceanographic contexts.

How to cite: Ehnis, M., Gutjahr, M., Menzel, D., Huang, H., Creac'h, L., Oetjens, A., Rieke, O., Herraiz Borreguero, L., Janout, M., Rickli, J., Frank, M., Tippenhauer, S., and Lippold, J.: Neodymium Cycling and Water Mass Structure in the Indian Sector of the Southern Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10619, https://doi.org/10.5194/egusphere-egu26-10619, 2026.

EGU26-11521 | ECS | Orals | OS1.6

A trapped East Greenland Current: Sea ice expansion during late MIS 6 in the eastern Fram Strait 

Monika Mikler, Pengyang Song, Jochen Knies, Gerrit Lohmann, Youngkyu Ahn, Seung-Il Nam, and Juliane Müller

The Fram Strait is a unique deep-sea gateway connecting the Arctic Ocean to the North Atlantic. Under modern conditions, the eastern Fram Strait remains largely ice-free due to the influx of warm Atlantic water via the West Spitsbergen Current (WSC). Conversely, the western Fram Strait is characterized by the export of cold, fresh Arctic water masses and sea ice from the central Arctic Ocean via the East Greenland Current (EGC), thereby impacting the North Atlantic thermohaline circulation. Paleoceanographic records, however, suggest radical departures from this oceanic regime during glacial periods (Geibert et al., 2021; Nørgaard-Pedersen et al., 2003).

Here, we present a high-resolution record of oceanographic conditions during Marine Isotope Stage (MIS) 6 using a sediment core KH14-GPC02, recovered from the eastern Fram Strait (77° 31' 22.7994" N, 8° 24' 4.9674" E) during Expedition CAGE19-3 in 2019.  Core KH14-GPC02 was analyzed for biomarker lipids, e.g., highly branched isoprenoids, sterols, and glycerol dialkyl glycerol tetraether lipids, providing the first complete, high-resolution records of sea-ice conditions and ocean temperature during the penultimate glacial maximum from this climatically critical region.

Our results reveal a two-phased evolution of sea-ice conditions in the eastern Fram Strait. Early MIS 6 was dominated by a marginal sea-ice cover with significant seasonal variability, as evidenced by high concentrations of the sea-ice biomarker IP25 and open-ocean biomarkers. From ~165 ka onward, however, a sharp decline in IP25 and open-ocean biomarkers signals a shift to perennial ice cover. To investigate the climatic drivers of this environmental transition, we conducted simulations with the complex Earth system model AWI-ESM. While lowered summer insolation and the closure of the Canadian Arctic Archipelago gateways contribute to regional cooling during glacial climates in the Fram Strait and Nordic Seas (e.g., Lofverstrom et al., 2022), our simulations demonstrate that these factors alone are insufficient to explain the perennial ice cover in the eastern Fram Strait during late MIS 6. Instead, we propose that the closure of the Denmark Strait, driven by ice‑sheet expansion, acted as a critical threshold to explain the heavy sea-ice cover in eastern Fram Strait during late MIS 6. This geographic blockage not only halted sea‑ice export through the Denmark Strait but also diminished the inflow of warm Atlantic water, fundamentally altering sea‑ice dynamics in the Arctic-Atlantic gateway. Our findings highlight the crucial – but often underestimated – role of oceanic gateways in regulating Arctic sea-ice extent during extreme glacial climates.

References

Geibert, W. et al., 2021. Nature 590, 97-102.

Lofverstrom, M. et al., 2022. Nature Geoscience 15, 482-488.

Nørgaard-Pedersen, N. et al., 2003. Paleoceanography 18, 1063.

 

How to cite: Mikler, M., Song, P., Knies, J., Lohmann, G., Ahn, Y., Nam, S.-I., and Müller, J.: A trapped East Greenland Current: Sea ice expansion during late MIS 6 in the eastern Fram Strait, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11521, https://doi.org/10.5194/egusphere-egu26-11521, 2026.

EGU26-13232 | ECS | Posters on site | OS1.6

Defining the States and Variability of Sea Ice via Marine Proxy Data Synthesis 

Georgia Melodie Hole, Helle Astrid Kjær, Nanna Andreasen, and Erin McClymont

Anthropogenic climate change is accentuated at high latitudes due to Polar Amplification, a process driven by interactions and feedback mechanisms among terrestrial, atmospheric, and oceanic systems. Arctic sea ice is in rapid decline while Antarctic sea ice has experienced recent extreme lows after relative stability, with global climatic and ecological responses and impacts. Multiple proxies have been developed for past sea ice reconstructions to assess modern trends and aid future forecasting. These include microfossil assemblages (dinocysts, foraminifera, ostracodes) and biomarker concentrations derived from ice-edge and open-water diatoms. Two sea ice biomarkers, IP25 (Ice Proxy with 25 carbon atoms) and IPSO25 (Ice Proxy for the Southern Ocean with 25 carbon atoms), can be used to produce semi-quantitative reconstructions of past sea ice extent when combined with phytoplankton derived biomarkers (e.g. phytosterols brassicasterol and dinosterol). However, there gaps remain in understanding past sea ice states and the critical processes that drive change, including at critical transitions that may provide insight into current and predicted future warming. We present an overview of synthesised sea-ice proxy records spanning key periods characterised by lower and higher than pre-industrial CO₂ background states: the Mid-Holocene (6ka; 8.2–4.2 ka BP), the Last Glacial Maximum (LGM; 21ka; ~ 19–23 ka), the Last Interglacial (LIG; 127ka; ~130–115 ka BP), and the Mid Pliocene Warm Period (mPWP: 3.264–3.025 Ma). These syntheses are feeding into model-data integration as a key component of the EU Horizon project Past-to-Future (P2F), which aims to radically advance our knowledge of past climatic conditions to better understand Earth’s climate response to different kinds of forcing. A better understanding of past sea ice states and stronger data–model integration are essential for improving our ability to anticipate the future trajectory of sea ice and its cascading effects on global climate.

How to cite: Hole, G. M., Kjær, H. A., Andreasen, N., and McClymont, E.: Defining the States and Variability of Sea Ice via Marine Proxy Data Synthesis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13232, https://doi.org/10.5194/egusphere-egu26-13232, 2026.

EGU26-14945 | Posters on site | OS1.6

Variability in biogeochemical Arctic outflow through Davis Strait 

Pete Brown, Edward Mawji, Stuart Painter, Jed Lenetsky, Carrie-Ellen Gabriel, Adrian Martin, Kumiko Azetsu-Scott, and Craig Lee

Polar ocean ecosystems are a key source of nutrients such as nitrogen (N) and phosphorus (P) to the rest of the world’s oceans. Climate change is already altering many processes affecting elemental cycling at the poles, but interruption of polar nutrient export could suppress global primary productivity and fisheries by around a quarter over multi-century timescales. It is thus essential to constrain both the mechanisms and variability of these fluxes, and their global implications.

The Arctic specifically exports an excess of P relative to N, equivalent to ~90% of the net phosphate flux to the Atlantic at 47°N, and supporting a significant fraction of North Atlantic N-fixation. Of the gateways into the Atlantic, Davis Strait has the strongest net southwards transport. A mooring array has been tracking volume and freshwater transports there since 2004, yet biogeochemical transports remain poorly quantified. To move towards addressing this gap, two autonomous water samplers were deployed at the western boundary of Davis Strait; targeting the P*-rich core of the Baffin Bay outflow (~100db) enabled the monitoring of nutrient transport of waters being exported into the North Atlantic, and the variability in their N:P relationship. 

Deployed in Ocober 2022, samples were collected at ~2 week intervals and analysed for inorganic and organic nutrients, oxygen isotopes and pH, forming the first two years of a dedicated biogeochemical time series of the western boundary outflow.  

Initial results show substantial chemical variability across all measured parameters, with a clear seasonal cycle in salinity-normalised nutrients and oxygen isotopes. When combined with velocity fields then concentration difference drive varialbity in the transports. While temperature and salinity also vary strongly on seasonal (and shorter) timescales, their cycles showed some temporal offsets, suggesting different underlying forcing mechanisms. Differences between the slope and off slope sites (a stronger amplitude in both concentrations and transports closer to the shelf)also highlight spatial structure in the exported water masses. 

Across the Straits then preliminary P* transport estimates underscore the dominant role of the western core in total nutrient export through Davis Strait. Early indications are of longer-term changes in N:P ratios in the outflow. Ongoing work will further refine transport estimates and assess implications for Arctic–Atlantic nutrient connectivity.

 

How to cite: Brown, P., Mawji, E., Painter, S., Lenetsky, J., Gabriel, C.-E., Martin, A., Azetsu-Scott, K., and Lee, C.: Variability in biogeochemical Arctic outflow through Davis Strait, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14945, https://doi.org/10.5194/egusphere-egu26-14945, 2026.

EGU26-17410 | ECS | Orals | OS1.6

Sea ice loss drives a regime shift in Arctic Ocean nitrogen biogeochemistry  

Marta Santos-Garcia, Raja Ganeshram, Laurent Oziel, Paul Dodd, Laura de Steur, Robyn Tuerena, and Colin Stedmon

The Arctic Ocean (AO) is changing very rapidly. Retreating sea-ice and the subsequent increase in light availability has significantly increased AO Net Primary Production (NPP). However, recent studies postulate that nutrients (and not light) now control NPP dynamics. We present observations from the Fram Strait (1998-2023) where this transition is revealed around 2009 as a sharp decline in fixed-nitrogen concentrations in the Polar Surface Water and an accompanying increase in Si:N ratios. We suggest that this represents a regime shift where fixed Nitrogen (N) has emerged as the main limiting factor for NPP in the contemporary AO. This reduction of N levels in the last decade may have resulted from increased benthic denitrification (BD) on the shelves. We investigate this by combining modelled BD rates and Lagrangian trajectories, which show a sharp increase in BD around 2009, with increasing contributions from the Chukchi and East Siberian shelves. We attribute this biogeochemical response to a drastic reduction in sea ice and circulation shift around this time. We suggest that Arctic climate change has led to a regime shift where low N levels resulting from increased loss of fixed N on the shelves now exert a tighter control on Arctic NPP. 

How to cite: Santos-Garcia, M., Ganeshram, R., Oziel, L., Dodd, P., de Steur, L., Tuerena, R., and Stedmon, C.: Sea ice loss drives a regime shift in Arctic Ocean nitrogen biogeochemistry , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17410, https://doi.org/10.5194/egusphere-egu26-17410, 2026.

EGU26-18273 | ECS | Posters on site | OS1.6

Synergistic Climate Modes Drive a Regime Shift in Physical-Biological Coupling in the Northern Antarctic Peninsula Region 

Suwen Ye, Zhaoru Zhang, and Petteri Uotila

The Northern Antarctic Peninsula (NAP) marine ecosystem is experiencing rapid environmental changes, yet the evolving relationships among atmospheric forcing, sea ice dynamics, and primary productivity remain poorly understood. This study investigates the interannual variability of summer chlorophyll-a (Chl-a) concentration and its physical drivers over the past two decades (2001–2024), utilizing multi-source satellite data and atmospheric reanalysis products. We identify a significant regime shift in climate-ecosystem interactions occurring around 2014.

Since 2014, major climate modes have shown concurrent trends: the Southern Annular Mode (SAM) accelerated towards a positive phase, while the Interdecadal Pacific Oscillation (IPO) shifted towards a negative phase. These combined trends led to a significant deepening of the Amundsen Sea Low (ASL), resulting in intensified regional winds (r=−0.79, p<0.01). This change in atmospheric circulation coincided with a rapid retreat of sea ice, marked by a significant increase in Ice-Free Days (IFD) in the NAP after 2014.

The significant change in climatic and physical conditions fundamentally altered the biological response patterns. Prior to 2014, the correlation between climate indices and summer Chl-a concentrations was weak, likely limited by the presence of sea ice cover. However, under low sea ice conditions after 2014, this association was notably strengthened. The correlation between the spring SAM index and summer Chl-a increased from 0.39 to 0.58 (p<0.1). The retreat of sea ice exposed the surface ocean directly to atmospheric forcing, enhancing the availability of irradiance and wind-driven vertical mixing. The enhanced mixing can facilitate the replenishment of limiting nutrients (e.g., iron) to the euphotic zone, thereby sustaining summer phytoplankton blooms. These findings suggest that the NAP ecosystem has entered a new state where productivity is tightly coupled with atmospheric dynamics.

How to cite: Ye, S., Zhang, Z., and Uotila, P.: Synergistic Climate Modes Drive a Regime Shift in Physical-Biological Coupling in the Northern Antarctic Peninsula Region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18273, https://doi.org/10.5194/egusphere-egu26-18273, 2026.

EGU26-19010 | Orals | OS1.6

Nonlinear Interactions of Timing and Amplitude Biases in Modeled Southern Ocean pCO2: The Roles of Dissolved Inorganic Carbon, Total Alkalinity, and Sea Surface Temperature 

Seth Bushinsky, Lionel Arteaga, Andrea Fassbender, Judith Hauck, Matthew Mazloff, Ivana Cerovečki, Peter Landschützer, Christian Rödenbeck, Christopher Danek, Anastasia Romanou, Paul Lerner, Alison Gray, and Sarah Schlunegger

The Southern Ocean is a major sink for atmospheric carbon dioxide and critical to the current and future carbon cycle. This net annual CO2 flux reflects the balance between strong seasonal variability characterized by opposing periods of winter outgassing and summer uptake. Using a simple framework, we evaluate how model biases in both the amplitude and timing of dissolved inorganic carbon (DIC) and total alkalinity (TA) and in the amplitude of sea surface temperature (SST) impact simulated pCO2. We examine seasonal CO2 fluxes and pCO2 south of the Subantarctic Front in 42 Earth System Model and three state estimate simulations. Only 11 of the 45 simulations have a seasonal pCO2 cycle with a correlation of ≥0.7 to observed pCO2, while 26 have a correlation of <0. Four of the well-correlated models accurately represent the seasonality of SST, DIC, and TA, while TA biases compensate for DIC or SST biases in the other seven. DIC and SST amplitude biases are related to mixed layer (MLD) biases, with shallow MLDs, especially in the summer, correlated with larger amplitude DIC and SST cycles than observed. The amplitude of seasonal Net Primary Production is correlated to DIC and TA timing. We provide input on the main adjustments needed to correct the simulated pCO2 seasonality in each of the evaluated models. These findings highlight the difficulty and importance of capturing the seasonal processes influencing the carbonate system to correctly model and predict the Southern Ocean carbon sink and its response to a changing climate. 

How to cite: Bushinsky, S., Arteaga, L., Fassbender, A., Hauck, J., Mazloff, M., Cerovečki, I., Landschützer, P., Rödenbeck, C., Danek, C., Romanou, A., Lerner, P., Gray, A., and Schlunegger, S.: Nonlinear Interactions of Timing and Amplitude Biases in Modeled Southern Ocean pCO2: The Roles of Dissolved Inorganic Carbon, Total Alkalinity, and Sea Surface Temperature, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19010, https://doi.org/10.5194/egusphere-egu26-19010, 2026.

EGU26-21652 | ECS | Posters on site | OS1.6

Reversal of Antarctic Intermediate Water trends triggered by sea ice decline 

Kaushik Mishra, Bishakhdatta Gayen, and Alberto C. Naveira Garabato

Antarctic Intermediate Water (AAIW) is a fundamental component of the global overturning circulation and a key determinant of the pycnocline structure. It is produced in the high-latitude Southern Ocean, where interactions between the ocean, atmosphere, and sea ice strongly shape its physical characteristics. From the late twentieth century through 2015, Antarctic sea ice underwent a sustained expansion of roughly 3% per decade. This prolonged growth enhanced the seasonal meltwater supply, increased surface stratification, and contributed to a gradual freshening of AAIW, whose effects were observed in the subtropical basins. Beginning in 2016, this pattern shifted abruptly. A sequence of unprecedented annual sea-ice losses signalled a rapid transition away from the earlier expansion phase. By combining Argo float measurements with satellite observations and reanalysis data, we demonstrate that this regime change is already affecting the properties of intermediate-depth water masses throughout the Southern Hemisphere. Our analysis indicates that, since 2016, the contribution of sea-ice meltwater has declined at a rate of up to 36 mSv per decade, a stark contrast to the pre-2015 increase of about 14 mSv per decade. This reduction in freshwater input has driven a concurrent increase in the density and salinity of AAIW, with core salinity rising by approximately 6×10-3 g kg-1 per decade. Together, these trends point to an emerging, hemispheric-scale adjustment of Southern Ocean–sourced water masses.

How to cite: Mishra, K., Gayen, B., and Naveira Garabato, A. C.: Reversal of Antarctic Intermediate Water trends triggered by sea ice decline, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21652, https://doi.org/10.5194/egusphere-egu26-21652, 2026.

CR4 – Frozen ground, debris-covered glaciers and geomorphology

EGU26-4085 | Orals | CR4.1

Net release of CO2 from thawing permafrost soil carbon predicted to occur earlier in this century 

Yi Xi, Philippe Ciais, Dan Zhu, Chunjing Qiu, Yuan Zhang, Shushi Peng, Simon P. K. Bowring, Daniel S. Goll, Pierre Friedlingstein, and Gustaf Hugelius

Accelerating permafrost thaw may mobilize vast stores of deep and frozen soil carbon (>3 m), releasing CO2 into the atmosphere. Yet, the magnitude of this release remains uncertain due to the absent deep carbon processes in current Earth system models (ESMs). Here, we use an updated ORCHIDEE-MICT model that explicitly simulates Yedoma formation during the Pleistocene and the transient development of northern peatlands during the Holocene to project northern (>30°N) carbon responses under climate change. Incorporating these deep, frozen carbon pools improves agreement with carbon cycle observations and reduces previously projected net CO2 uptake by 47–74 Pg C between 1900 and 2100 across three future scenarios. Under high-emission pathways, the northern soil carbon balance shifts from a net sink to a net source of up to 32 Pg C, advancing the reversal predicted by the original model earlier in the 21st century. This earlier reversal is primarily driven by accelerated deepening of the active layer after mid-century, exposing more previously frozen carbon, particularly from Yedoma. Consistent with field data, our model shows that colder soils retain more labile carbon—contrary to assumptions in many IPCC models, which helps explain their prediction of a continuous carbon sink. Our results highlight the need to represent both the quantity and quality of permafrost carbon in ESMs to improve projections of permafrost–climate feedbacks.

How to cite: Xi, Y., Ciais, P., Zhu, D., Qiu, C., Zhang, Y., Peng, S., Bowring, S. P. K., Goll, D. S., Friedlingstein, P., and Hugelius, G.: Net release of CO2 from thawing permafrost soil carbon predicted to occur earlier in this century, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4085, https://doi.org/10.5194/egusphere-egu26-4085, 2026.

Permafrost is extensively distributed across the Qinghai-Tibet Plateau (QTP) in China and is interspersed with numerous streams, rivers, and lakes, forming a highly sensitive cryo-hydrogeological environment. Beneath these aquatic systems, permanently unfrozen zones, known as taliks, commonly develop within the permafrost and play a critical role in regulating hydraulic connectivity and water exchange between groundwater and surface water. As such, river-talik systems exert a strong influence on regional water resources, river discharge regimes, and the stability of engineering infrastructure. Nevertheless, the functioning and dynamics of river-talik systems in discontinuous permafrost regions remain complex and insufficiently understood. During the summer season, when taliks remain hydraulically connected to the riverbed, groundwater flow through taliks can sustain river baseflow, thereby influencing seasonal water availability and downstream water resources. In contrast, during winter, progressive refreezing of the riverbed disrupts this hydraulic connection, resulting in groundwater pressure accumulation within aquifers at talik constrictions. Elevated groundwater pressure may fracture the overlying ice cover, allowing supra-permafrost groundwater to discharge onto river floodplains and form extensive icings. These processes not only alter winter runoff pathways but may also inundate adjacent land and infrastructure corridors. In addition, ongoing permafrost degradation beneath riverbeds can induce differential ground settlement, which poses significant risks to bridge foundations, embankments, and other critical infrastructure in cold regions. To investigate the cryo-hydrogeological characteristics and engineering implications of a complex river-talik system in a discontinuous permafrost region of the QTP, a comprehensive field-based approach was employed, integrating continuous monitoring of ground temperature, surface temperature, and hydraulic head with electrical resistivity tomography (ERT) surveys. The presence of flowing river water enhances subsurface heat storage beneath the riverbed, substantially delaying riverbed freezing during autumn and early winter. Moreover, the formation, thickening, and lateral expansion of icings during winter provide an additional thermal buffer. Together, these processes maintain ground temperatures above 0 °C at depth throughout the year, resulting in the development of an approximately 2 m thick talik beneath the riverbed. ERT inversion results further identify both supra-permafrost taliks and taliks penetrating through the permafrost. The river talik exhibits a complex three-dimensional geometry, with cross-sectional dimensions varying along the channel and extending locally above or intermittently through the permafrost. Furthermore, the warm permafrost underlying the talik retains partial permeability, allowing limited groundwater flow within the permafrost matrix. Collectively, these characteristics give rise to intricate local-scale cryo-hydrogeological processes that strongly affect groundwater-surface water interactions, winter river dynamics, and the long-term stability of infrastructure in permafrost regions.

How to cite: Liu, W.: River Talik Development and Its Implications for Cryo-Hydrogeological Processes and Infrastructure in Permafrost Regions on the Qinghai-Tibet Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4328, https://doi.org/10.5194/egusphere-egu26-4328, 2026.

EGU26-5967 | ECS | Posters on site | CR4.1

Seasonal variation of hydrologic connectivity for High Arctic stream segments 

Jonas Eschenfelder, Shawn M. Chartrand, and A. Mark Jellinek

In the High Arctic, new channel networks are developing relatively rapidly within 10s of years, typically attributed to exteneded thaw seasons under climate change and late season permafrost loss. During the 2024 field season on Tallurutit (Devon Island), we visited a developing channel network where relatively flat pools are connected by steeper channelised segments which exhibit evidence of recent gravel and sand transport. However, despite visiting during a storm event, we did not observe active sediment transport and only limited surface-water runoff. This brings up the question: How does the hydrologic connectivity between channel segments and surface runoff fraction change across a thaw season?

We developed a new box model that couples surface and subsurface water flow between pools conserving enthalpy to explore the hydrologic response of an analogue landscape segment across a thaw season. Using this model, we first use synthetic rainevents to identify the key factors modulating the hydrologic response and then use new weather data from Tallurutit and historic climate data to explore when surface water erosion is likely to occur under typical climate conditions and for future climate scenarios.

Subjecting the landscape to the same magnitude-duration rainevent in the early versus late thaw season shows that surface water runoff fraction is greatest early in the thaw season as the shallow thaw front limits subsurface water storage. This results in successive overspill events that rapidly transport water across pools and promote erosion. In the late thaw season, subsurface water storage dominates and pools are connected via subsurface water flow. As a result surface water flow and resultant erosion is minimised. We summarise a key implication of our work through a reservoir response time that depends on the bed permeability, pool length, and thaw depth which modulates whether a pool will dampen a hydrologic signal or transmit it downstream.

Combined with grain-scale laboratory experiments which show that bed erodibility is inversely proportional to thaw depth, this work suggests that the formation and evolution of channel networks in the High Arcitc is primarily driven by early season discharge events. Under climate change, the frequency and magnitude of early season rainstorms and heatwaves, resulting in rapid snowmelt, are becoming more common. This suggests that the observed rapid channelisation in the High Arctic is related to early season climate extremes, instead of long-term warming averages and late season permafrost loss.

How to cite: Eschenfelder, J., Chartrand, S. M., and Jellinek, A. M.: Seasonal variation of hydrologic connectivity for High Arctic stream segments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5967, https://doi.org/10.5194/egusphere-egu26-5967, 2026.

EGU26-8385 | Orals | CR4.1

Abrupt changes in subarctic stream chemistry linked to permafrost thaw and sulfide mineral oxidation 

Matthew Lindsay, Elliott Skierszkan, Andras Szeitz, and Sean Carey

Acidification and metal mobilization linked to sulfide mineral oxidation pose an urgent risk to water quality and ecosystem health in thawing permafrost regions. Over the past six years, we have observed large increases in sulfate and metal concentrations and fluxes coupled with notable pH decreases in several headwater streams in the Tombstone Waters Observatory, Yukon, Canada. Field observations and satellite imagery reveal the emergence of acidic seepage zones characterized by extensive vegetation dieback and ochreous mineral precipitation. This seepage can exhibit pH < 3 and sulfate concentrations up to 5000 mg L-1, with metal (e.g., Fe, Al, Mn, Ni, Zn) concentrations ranging from 10s to 100s of mg L-1 and often exceeding water quality criteria. Subsequent pH buffering along groundwater discharge and stream mixing zones drives extensive precipitation of Al and Fe (oxyhydr)oxide and (hydroxy)sulfate phases, which influence metal transport and are visible many kilometers downstream. Notable increases in sulfate concentrations for major downstream rivers (e.g., Klondike, Ogilvie, Peel) show that coupled biogeochemical and hydrological processes in headwater catchments can have widespread impacts. Moreover, the growing occurrence of acidic seepage zones and ochreous mineral precipitates suggests impacts of permafrost thaw and sulfide mineral oxidation represent a substantial long-term risk to subarctic stream chemistry. Our ongoing research at the Tombstone Waters Observatory aims to advance understanding of the complex coupled processes influencing stream water chemistry in thawing permafrost regions. 

How to cite: Lindsay, M., Skierszkan, E., Szeitz, A., and Carey, S.: Abrupt changes in subarctic stream chemistry linked to permafrost thaw and sulfide mineral oxidation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8385, https://doi.org/10.5194/egusphere-egu26-8385, 2026.

EGU26-9260 | ECS | Orals | CR4.1

Impact of Soil Moisture on Carbon Cycle Changes in Permafrost Regions in CESM2 

Jin-Hyuk Mun, Hanna Lee, Danbi Lee, Yechul Shin, and Jong-Seong Kug

Permafrost regions store vast amounts of soil carbon, and warming-driven thaw can enhance microbial decomposition and carbon dioxide release, strengthening the permafrost carbon feedback. Although this feedback has been widely studied under continued warming, the processes governing its magnitude and persistence remain highly uncertain. Here we use the Community Earth System Model version 2 (CESM2) to examine permafrost carbon-cycle dynamics under both warming and mitigation, and apply multiple regression to quantify the controls on net biome production. We identify soil moisture as a key regulator of carbon cycle dynamics. Thaw-driven increases in liquid soil water enhance plant photosynthesis, but more strongly accelerate microbial decomposition, shifting ecosystems toward net carbon release and reducing net biome production. Sensitivity to soil moisture is strongly heterogeneous, with the largest response in central Siberia where high litter carbon coincides with relatively low climatological soil moisture, whereas North America shows weaker sensitivity under a wetter background state. Soil moisture also delays recovery after mitigation by slowing permafrost refreezing and sustaining anomalously wet soils during the net-zero period. This maintains elevated heterotrophic respiration and prolongs negative net biome production even after mitigation. In conclusion, our results show that soil moisture can amplify and sustain permafrost carbon losses along mitigation pathways, highlighting improved representation of coupled soil hydrology and permafrost processes as a priority for reducing uncertainty in future carbon budget assessments.

How to cite: Mun, J.-H., Lee, H., Lee, D., Shin, Y., and Kug, J.-S.: Impact of Soil Moisture on Carbon Cycle Changes in Permafrost Regions in CESM2, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9260, https://doi.org/10.5194/egusphere-egu26-9260, 2026.

EGU26-9850 | Orals | CR4.1

Compound effects of permafrost thaw, vegetation dynamics, and increasing CO2 alter carbon budget of the permafrost zone 

Thomas Kleinen, Philipp de Vrese, Helena Bergstedt, and Victor Brovkin

Under changing climatic conditions, the Arctic is undergoing massive changes. Due to Arctic amplification, the Arctic is warming faster than any other region on Earth. The combination of warming and CO2 fertilization leads to increases in productivity and changes in vegetation composition, with shrubs invading the Tundra, and trees also shifting northwards. At the same time, permafrost thaws, adding previously frozen carbon deposits to the active carbon cycle. The net carbon balance resulting from all of these coupled processes is less clear than one might think and requires an integrated modelling approach.

We use ICON-Land, the land surface model of the ICON Earth System Model, to investigate changes in the carbon cycle of the permafrost region. We have extended the soil carbon model YASSO by introducing a vertical dimension in order to consider carbon storages in deeper frozen soil layers. Furthermore, we are considering Arctic-specific shrub PFTs in our dynamic vegetation scheme in order to represent the changes in vegetation composition expected in a changing climate, thus allowing a complete assessment of carbon cycle changes.

We initialise the soil C pools for the preindustrial climate state from the Northern Circumpolar Soil Carbon Database to insure initial C pool sizes close to measurements. We then determine changes in vegetation composition and soil C storage in transient model experiments following historical and future climate changes under RCPs 2.6, 4.5, and 8.5. Based on these experiments, we quantify the greenhouse gas balance under future climatic conditions. While the permafrost soils lose carbon in all scenarios, productivity increases, especially if the vegetation can adapt to the changed climatic conditions, leading to lower carbon release.

How to cite: Kleinen, T., de Vrese, P., Bergstedt, H., and Brovkin, V.: Compound effects of permafrost thaw, vegetation dynamics, and increasing CO2 alter carbon budget of the permafrost zone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9850, https://doi.org/10.5194/egusphere-egu26-9850, 2026.

EGU26-10212 | ECS | Posters on site | CR4.1

Stochastic Modelling of Thermokarst Lakes 

Constanze Reinken, Victor Brovkin, Philipp de Vrese, Ingmar Nitze, Helena Bergstedt, and Guido Grosse

Thermokarst lakes are widespread and dynamic features of ice-rich permafrost landscapes. They accelerate permafrost thaw, enhance methane production, and alter soil hydrology as well as energy and water exchanges between land and atmosphere. These effects can alter local and global climate. But despite their important role in the climate sysem, thermokarst lakes are largely absent from Earth system models (ESMs), because deterministic and physics-based modelling approaches require extensive high-resolution ground-ice data that are not available. To close this gap, we develop a probabilistic modeling framework that represents lake dynamics as stochastic processes and can be parameterized using remote sensing data. The model has the potential to provide evolving Arctic water-area fractions and lake-size distributions that can be coupled to ESMs, improving the representation of permafrost dynamics and high-latitude carbon emissions under climate change.

How to cite: Reinken, C., Brovkin, V., de Vrese, P., Nitze, I., Bergstedt, H., and Grosse, G.: Stochastic Modelling of Thermokarst Lakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10212, https://doi.org/10.5194/egusphere-egu26-10212, 2026.

EGU26-10730 | Posters on site | CR4.1

Analytical–statistical models (ASMs) for mean annual permafrost table temperature and active-layer thickness 

Tomáš Uxa, Filip Hrbáček, and Michaela Kňažková

Mean annual permafrost table temperature (MAPT) and active-layer thickness (ALT) are key variables for assessing the thermal regimes of permafrost and active layer and their responses to climate changes. Models for estimating MAPT and ALT have typically been forced by air or ground temperatures and some ground physical properties. While temperature measurements are relatively widely available and reliable, ground physical properties are frequently unavailable or unrepresentative and therefore need to be estimated, which introduces uncertainties into model outputs.

Hence, we devised two simple analytical−statistical models (ASMs) for estimating MAPT and ALT, which are driven solely by pairwise combinations of freezing and thawing indices in the active layer. We tested the models at the total of 55 sites in the Earth's major permafrost regions comprising five different ground surface covers and four permafrost zones where the models showed the total mean errors of less than 0.05 °C for MAPT and 9 % for ALT. Besides, the models can also be used to establish typical values of some ground physical parameters for MAPT and ALT estimates. We believe that ASMs can find useful applications in permafrost and active-layer modelling under a wide range of climates, ground surface covers, and ground physical conditions.

 

Acknowledgement

The research was funded by the Czech Science Foundation (project numbers GM22-28659M and GA25-18272S) and by the Ministry of Education, Youth and Sports (project number LL2505).

How to cite: Uxa, T., Hrbáček, F., and Kňažková, M.: Analytical–statistical models (ASMs) for mean annual permafrost table temperature and active-layer thickness, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10730, https://doi.org/10.5194/egusphere-egu26-10730, 2026.

EGU26-12648 | Posters on site | CR4.1

Mechanism of thaw settlement induced by segregated ice melting based on a visualizing study 

Zheng Wang, Zixuan Huo, and Chi Zhang

The melting of segregated ice in ice-rich frozen soils is a primary driver of soil structural instability and thaw settlement, yet the dynamic morphological evolution of segregated ice and its quantitative linkage to thaw settlement remain poorly understood. To address this issue, a series of physical model experiments were conducted using a self-developed visualized thaw settlement experimental platform for ice-rich frozen soils. Thus, the different surface thawing temperatures (5 °C, 7 °C, and 10 °C) , multiple particle-size gradation schemes (G-I to G-V), and different external load levels (0.5 kPa, 1.0 kPa, and 1.5 kPa) were introduced to investigate the influence of temperature, gradation, and pressure on segregated ice melting and thaw settlement behavior. The results indicate that the melting process of segregated ice can be divided into a rapid phase-change stage and a stable thaw settlement stage. An increase in surface thawing temperature significantly shortens the duration of the phase-change stage and enhances downward migration of liquid water toward the unfrozen zone, resulting in a pronounced increase in thaw settlement. Particle-size gradation regulates moisture accumulation and migration by modifying pore structure and capillary force intensity; segregated ice is more readily formed in fine-grained soils, which exhibit a higher risk of thaw settlement after melting. External loading has a limited influence on the phase-change pattern; however, by increasing pore water pressure, it significantly intensifies settlement deformation during the stable stage. Pore structure collapse induced by segregated ice melting dominates the rapid settlement stage, whereas pore water drainage and soil skeleton reorganization govern deformation during the stable thaw settlement stage.

How to cite: Wang, Z., Huo, Z., and Zhang, C.: Mechanism of thaw settlement induced by segregated ice melting based on a visualizing study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12648, https://doi.org/10.5194/egusphere-egu26-12648, 2026.

EGU26-12875 | Orals | CR4.1

Permafrost Experimental Protocol within the Tipping Point Modelling Intercomparison Project (TIPMIP) 

Goran Georgievski, Victor Brovkin, Eleanor Burke, Jan Nitzbon, Norman Steinert, Delphine Tardif, Donovan Dennis, Sina Loriani, Jonathan Donges, and Ricarda Winkelmann

Within the Tipping Point Modeling Intercomparison Project (TIPMIP; www.tipmip.org), we outline a coordinated experimental protocol designed for standalone land surface models (LSMs) as well as coupled Earth System Models (ESMs). The protocol targets key questions on permafrost feedbacks, thresholds, timescales, abrupt versus gradual, and irreversible changes, and interactions with other tipping elements, aiming to quantify plausible landscape transformations, associated greenhouse gas emissions, and their impacts on global energy, carbon, and hydrological cycles, as well as large scale circulation.

Building on TIPMIP-ESM, the TIPMIP-permafrost Tier 1 experiments, defined as the core, priority experiments required for MIP participation, aim to use LSMs to quantify the extent to which permafrost area, ground ice volume, and soil carbon stocks exhibit path dependent behavior and reversibility when subjected to idealized warming, stabilization, and subsequent cooling phases. This includes evaluating whether the permafrost returns to its initial state as temperatures decline, or the extent to which certain changes, such as area loss, carbon redistribution, hydrological reorganization, or ground subsidence, persist despite cooling and thus remain effectively irreversible over time scales spanning a century to a several hundred years. In addition, during the stabilization phase we will examine whether permafrost degradation continues even after warming ceases. This involves assessing time lagged thaw response, identifying critical thresholds that may trigger rapid acceleration of degradation, and determining whether internal processes, such as shifts in soil moisture, ground subsidence and thermokarst lake formation, or carbon redistribution, amplify change through self reinforcing feedbacks. The emergence of such behaviors would indicate nonlinear system dynamics and a heightened susceptibility to tipping point transitions.

Additional sensitivity experiments (Tier 2), aimed at understanding and quantifying specific processes that could induce permafrost tipping, will apply idealized forcing. The focus is on altering hydrologic conditions and modifying surface properties (e.g., vegetation, albedo, thermokarst lake distribution) to explore how these factors influence the onset and dynamics of tipping behavior.

Tier 3 experiments, also sensitivity oriented, investigate the coupling between permafrost dynamics and other climate tipping elements using ESMs, for example, assessing the consequences of an AMOC collapse for high latitude permafrost stability, as well as the broader Earth system impacts of abrupt permafrost tipping.

How to cite: Georgievski, G., Brovkin, V., Burke, E., Nitzbon, J., Steinert, N., Tardif, D., Dennis, D., Loriani, S., Donges, J., and Winkelmann, R.: Permafrost Experimental Protocol within the Tipping Point Modelling Intercomparison Project (TIPMIP), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12875, https://doi.org/10.5194/egusphere-egu26-12875, 2026.

EGU26-12991 | ECS | Orals | CR4.1

Periglacial Regions as Hotspots of Oxidative Weathering that Drive Deglacial Acceleration of Rock Carbon Release 

Alasdair Knight, Chris Stokes, Laura Stevens, Julie Cosmidis, Jemma Wadham, Edward Tipper, Lucy Wright, and Robert Hilton

Cryospheric retreat associated with deglaciation and permafrost thaw exposes previously stable carbon reservoirs to active biogeochemical cycling. While substantial effort has focused on constraining greenhouse gas emissions from thawing soil organic matter, many cryospheric environments also host large carbon stocks within bedrock and regolith, whose contribution to carbon-climate feedbacks remains poorly quantified. Mobilisation of these carbon stocks can enhance CO2 release to the atmosphere via an acceleration of sulphide mineral and rock-derived organic carbon oxidation. Multi-decadal increases in riverine sulphate concentrations across the Arctic, together with growing reports of “rusting rivers”, provide compelling evidence for a direct link between permafrost degradation and enhanced oxidative weathering. However, the magnitude, spatial distribution, and climatic significance of this feedback remain poorly constrained.

Here, we quantify the impact of cryospheric retreat on oxidative weathering through a field investigation spanning five valleys in Svalbard underlain by contrasting lithologies. Surface water geochemistry and discharge measurements collected from glacier termini to valley bottoms reveal that CO2 release from geological carbon stocks is sustained—and in some cases amplified—downstream of glacier margins. These observations indicate that enhanced oxidative weathering is not confined to subglacial environments but persists across regions subject to paraglacial processes. This improved spatial understanding of oxidative weathering is used to inform a forward model of carbon release from geological reservoirs resulting from permafrost thaw and and ice-sheet retreat, focused on the last deglaciation. Together, our results demonstrate that cryospheric retreat can enhance carbon release from geological reservoirs, representing a previously under-constrained positive feedback on the Earth system with implications for both past climate transitions and ongoing cryospheric retreat.

How to cite: Knight, A., Stokes, C., Stevens, L., Cosmidis, J., Wadham, J., Tipper, E., Wright, L., and Hilton, R.: Periglacial Regions as Hotspots of Oxidative Weathering that Drive Deglacial Acceleration of Rock Carbon Release, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12991, https://doi.org/10.5194/egusphere-egu26-12991, 2026.

EGU26-13227 | ECS | Posters on site | CR4.1

Post-glacial emergent permafrost processes within coastal and paleo-lagoon settings on Svalbard 

Michael Angelopoulos, Katharina Boie, Maximilian Rau, Maike Offer, Saskia Eppinger, Ernst Hauber, Michael Zanetti, Cynthia Sassenroth, Andreas Johnsson, Harald Hiesinger, Nico Schmedemann, Pier Paul Overduin, Julia Boike, Sebastian Westermann, Bernard Hallet, and Michael Krautblatter

Saline permafrost exists beneath shallow shelf seas, coastal plains shaped by past marine transgressions, and post-glacially uplifted landscapes that were once submerged. Salinity influences the freezing point and mechanical strength of permafrost; it is, therefore, a critical parameter for assessing its stability. On Svalbard, the Kvadehuksletta region northwest of Ny-Ålesund features a diverse landscape comprising raised beach terraces, lagoons, paleo-lagoons (now lakes), and surface seeps. Our research aims to decipher how marine sediments transform after emergence. We hypothesize that ice formation during permafrost aggradation produces a porewater salinity gradient that triggers the downwards migration of salt in slowly uplifting sediments that are weakly susceptible to groundwater flushing. Sufficient salt build-up may lead to the formation of cryopegs. Cryopegs, a type of talik, are unfrozen layers or pockets within permafrost that persist at subzero temperatures due to their elevated salt content. In summer 2024 and 2025, we carried out several electrical resistivity tomography (ERT) profiles, including three profiles (ranging from 800 to 2300 m in length) perpendicular to the coastline. The westernmost profile (collected in 2025) intersected a dynamic lagoon that was connected to the sea in 2024 but became completely cut off in 2025 by storm-surge deposits. To help delineate frozen and unfrozen permafrost conditions, electrical resistivity-temperature analyses of field samples collected from shallow cores (down to 2.5 m) are currently underway. Laboratory tests indicate that the near-surface marine clays adjacent to the lagoon have low resistivities (< 10 Ωm) when thawed and freezing point temperatures down to -1.6 °C. The field samples are also being analysed for porewater chemistry (electrical conductivity, cations & anions, pH, stable water isotopes) and basic sedimentological properties like grain size. At two coring sites (1 paleo-lagoon, 1 beach setting), an annual ground temperature time series was also collected between field seasons. While the physical and electrical properties of the marine sediments are important to establish, so is their thickness. To potentially provide additional information on the depth to bedrock along selected ERT profile segments, we conducted multiple seismic refraction tomography (SRT) surveys (115 m length) in 2025 using a sledgehammer as an energy source. The synthesis of all datasets to describe uplifted permafrost is work in progress, but preliminary conclusions suggest that cryopeg occurrence is most likely in low-lying coastal areas characterized by warm permafrost, occasional seawater submergence, and saline marine clays with low hydraulic conductivity.

How to cite: Angelopoulos, M., Boie, K., Rau, M., Offer, M., Eppinger, S., Hauber, E., Zanetti, M., Sassenroth, C., Johnsson, A., Hiesinger, H., Schmedemann, N., Overduin, P. P., Boike, J., Westermann, S., Hallet, B., and Krautblatter, M.: Post-glacial emergent permafrost processes within coastal and paleo-lagoon settings on Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13227, https://doi.org/10.5194/egusphere-egu26-13227, 2026.

EGU26-13457 | ECS | Orals | CR4.1

Global permafrost evolution 1960–2100: A new high-resolution model assessing past change and projecting scenario-based futures. 

Harley R. McCourt, Matthew J. Westoby, Stuart A. Dunning, Sammie Buzzard, and Michael Lim

Permafrost is experiencing rapid and widespread degradation in response to atmospheric warming, with profound implications for landscape stability, infrastructure planning, hazard assessment, and carbon-climate feedback. While probabilistic approaches to global permafrost modelling exist (Gruber, 2012), no framework currently spans the 1960–2020 period, a critical window encompassing the acceleration of anthropogenic climate change and the most pronounced observed warming in permafrost regions. Here, we present GRAPE-60 (Global ReAnalysis-driven Permafrost Extent estimate over a 60-year period), a high-resolution equilibrium-based permafrost model that integrates modern reanalysis datasets (ERA5 and JRA-55) with digital elevation models (ASTER and SRTM) to quantify global permafrost evolution from 1960 to 2020 and extend this framework to project future change under differing climate scenarios. Through systematic evaluation of multiple model configurations against borehole observations, we identify ERA5-ASTERDEM as the optimal combination, achieving an area under the receiver operating characteristic curve of 0.96 for historical periods. Independent comparison of the downscaled air temperatures product against ESA CCI satellite-derived land surface temperature (1996–2020) yielded a mean bias of +0.79°C (σ = 1.64°C), demonstrating agreement within the uncertainty bounds of the reference dataset. Our historical results reveal a net global permafrost loss of 2.49 × 10⁶ km² (8.9% of the exposed land area) between 1960 and 2020, with marked spatial patterns: continuous permafrost zones contracted by 21% while isolated patches expanded by 12%, indicating widespread degradation and fragmentation. To project future permafrost trajectories, we utilise GRAPE-60 as a spin-up and bias-correct temperature forcings from selected CMIP6 Earth System Models under SSP1-2.6, 2-4.5, 3-7.0, and 5-8.5 scenarios. Preliminary results reveal scenario-dependent pathways ranging from near-stabilisation under aggressive mitigation to substantial additional losses under high-emission futures. This work provides the first high-resolution, multi-decadal reconstruction of global permafrost evolution 1960-2020 and establishes a methodological framework for tracking and projecting future changes in this critical and rapidly transforming component of the cryosphere.

How to cite: McCourt, H. R., Westoby, M. J., Dunning, S. A., Buzzard, S., and Lim, M.: Global permafrost evolution 1960–2100: A new high-resolution model assessing past change and projecting scenario-based futures., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13457, https://doi.org/10.5194/egusphere-egu26-13457, 2026.

EGU26-13913 | Posters on site | CR4.1

Improved Process Understanding Using  Stand-alone Land Surface Models in Simulating Permafrost 

Bodo Ahrens, Zhicheng Luo, Mittal Parmar, and Danny Risto

Land surface models (LSMs) still exhibit widespread deficiencies in frozen soil regions, particularly in overestimating soil temperature responses to air temperature under snow cover and in simulating soil moisture dynamics (see, e.g., Luo et al (2025)). Analysis of CMIP6 simulations reveals that, in frozen soil areas, the influence of LSMs on coupled climate model results is comparable in magnitude to that of atmospheric forcing. Moreover, compensating effects between land and atmosphere components often lead to apparently better performance in coupled simulations than in offline LSM experiments. This compensation poses a risk that structural deficiencies in LSMs may remain obscured when evaluating coupled model performance.

To identify specific weaknesses in current LSM formulations, we conduct offline simulations using three land surface models—CLM5, TERRA standalone, and JSBACH—at permafrost observation sites, including Bayelva (Svalbard) and Samoylov (Lena River Delta). The models are driven by meteorological forcing derived from the WATCH Forcing Data methodology applied to ERA5 (WFDE5), which is further bias-corrected to the sites using in situ observations.

We evaluate simulated snow water equivalent, soil temperature, soil moisture, and surface energy fluxes against observations, complemented by targeted sensitivity experiments. This approach aims to diagnose the key processes responsible for model biases in permafrost regions and to assess potential pathways for improving land surface model performance under cold-region conditions.

 

Zhicheng Luo, Risto, D., B. Ahrens (2025) Assessing Climate Modeling Uncertainties in the Siberian Frozen Soil Regions by Contrasting CMIP6 and LS3MIP. The Cryosphere, 19, 6547–6576. https://doi.org/10.5194/tc-19-6547-2025

How to cite: Ahrens, B., Luo, Z., Parmar, M., and Risto, D.: Improved Process Understanding Using  Stand-alone Land Surface Models in Simulating Permafrost, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13913, https://doi.org/10.5194/egusphere-egu26-13913, 2026.

EGU26-14309 | ECS | Posters on site | CR4.1

Millennial-Scale Land–Climate Interactions Using a Deepened CLM5 Lower Boundary: Permafrost Evolution, Vegetation Dynamics, and Coupled Feedback in CESM2 

Meisam Heidari, Hugo Beltrami, Francesco S. R. Pausata, François Counillon, and J. Fidel González Rouco

Permafrost evolution and subsurface thermal dynamics play a key role in the climate system, yet their representation in Earth System Models (ESMs) remains constrained by shallow soil configurations. This study investigates millennial-scale land–climate interactions using simulations with the Land Surface Model CESM2/CLM5 employing a modified deep lower boundary extending to 500 m, alongside the standard 43 m configuration. Simulations span 500–2014 CE and are driven by boundary conditions obtained from two NorESM1-F PARCIM experiments over the same time interval. These experiments follow PMIP last-millennium protocols and include prescribed variations in solar irradiance, volcanic forcing, and greenhouse gas concentrations, while anthropogenic aerosol and land cover are held fixed at pre-industrial conditions. Two solar forcing reconstructions are used, representing low and high solar variability, enabling assessment of how land model depth and natural external forcing shape subsurface thermal states, permafrost extent, active-layer thickness, and soil carbon evolution on centennial to millennial timescales. Simulations using the deep land configuration exhibit reduced variability in the simulated permafrost area during the pre-industrial period (500–1850 CE) relative to the standard shallow configuration. Evaluation against observational and reanalysis-based datasets over 1997–2021 indicates closer agreement for the high solar variability forcing than for the low variability forcing with respect to permafrost extent and subsurface thermal conditions. High-latitude vegetation responses are further explored using modified CLM-FATES configurations. Finally, selected CAM–CLM coupled simulations are used to assess land–atmosphere feedback and to examine how differences between deep and shallow land states propagate into future projections under SSP scenarios from 2015 to 2100.

How to cite: Heidari, M., Beltrami, H., Pausata, F. S. R., Counillon, F., and Rouco, J. F. G.: Millennial-Scale Land–Climate Interactions Using a Deepened CLM5 Lower Boundary: Permafrost Evolution, Vegetation Dynamics, and Coupled Feedback in CESM2, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14309, https://doi.org/10.5194/egusphere-egu26-14309, 2026.

EGU26-14668 | Orals | CR4.1

Can soil carbon content explain inter-site differences in carbon flux magnitude across the permafrost region? 

Frans-Jan W. Parmentier, Luca Belelli Marchesini, Christian Wille, Gustaf Hugelius, Mathias B. Siewert, Mika Aurela, Julia Boike, Torben R. Christensen, Han Dolman, Thomas Friborg, Mathias Goeckede, Geert Hensgens, David Holl, Ko van Huissteden, Lars Kutzbach, Norbert Pirk, Torsten Sachs, Narasinha Shurpali, Yuqing Zhao, and Peter Kuhry

The permafrost region holds vast amounts of carbon which, upon thaw, may be released to the atmosphere as CO2 through enhanced decomposition. While links between soil carbon content and respiration have been shown by, for example, numerous incubation studies, it remains challenging to establish similar relationships from in-situ data collected in the field – especially at the large landscape-scale of eddy covariance towers. Part of the reason is the high heterogeneity of Arctic landscapes, combined with frequently shifting footprint distributions, and general lack of detailed soil carbon data that make it difficult to separate the signal from the noise. In this study, therefore, we combine detailed surveys of soil carbon content with high resolution footprint analyses to explore whether inter-site differences in carbon fluxes across ten sites spanning the Arctic can be explained by soil carbon content. Soil carbon data at each site was collected across dominant landforms and analyzed with depth. At 5 sites, these data were further developed into high resolution soil carbon maps. At the remaining sites, spatially weighted estimates of soil carbon content were determined proportionally to dominant landforms. Net CO2 fluxes collected by the towers were processed according to the same pipeline and partitioned into GPP and ecosystem respiration. These fluxes were related to the amount of soil carbon in the active layer at dominant landforms through a spatially explicit footprint analysis. Our preliminary results suggest that active layer soil carbon storage is a strong predictor of inter-site differences in ecosystem respiration during the growing season. This study will further explore the robustness of this relationship across the Arctic and throughout the year.

How to cite: Parmentier, F.-J. W., Belelli Marchesini, L., Wille, C., Hugelius, G., Siewert, M. B., Aurela, M., Boike, J., Christensen, T. R., Dolman, H., Friborg, T., Goeckede, M., Hensgens, G., Holl, D., van Huissteden, K., Kutzbach, L., Pirk, N., Sachs, T., Shurpali, N., Zhao, Y., and Kuhry, P.: Can soil carbon content explain inter-site differences in carbon flux magnitude across the permafrost region?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14668, https://doi.org/10.5194/egusphere-egu26-14668, 2026.

EGU26-15161 | Posters on site | CR4.1

Permafrost cloud feedback 

Philipp de Vrese, Tobias Stacke, Veronika Gayler, and Victor Brovkin

Rising temperatures in the northern permafrost zone are profoundly altering key surface and subsurface processes, triggering important climate feedbacks. The most prominent of these is the accelerated decomposition of formerly frozen soil organic matter, leading to the release of carbon into the atmosphere. In addition, changes in surface and soil hydrology may influence regional and global climate through cloud radiative effects. The thawing of previously impervious soil layers increase hydrologic connectivity, thereby enhancing drainage and increasing landscape drying. This process limits evapotranspiration during the spring and summer months, reducing the formation of low-altitude clouds throughout the snow-free season. The decrease in summertime cloud cover, in turn, allows for greater shortwave absorption at the surface, amplifying temperatures and further accelerating permafrost degradation.

In this study, we investigate recent trends in cloud cover and soil moisture to identify potential signals of a permafrost-cloud feedback in observational and reanalysis datasets. While substantial disagreement exists between data sources regarding the signal strength and spatial patterns, we observe a consistent increase in the correlation between summertime cloud cover and soil moisture over recent decades, coupled with widespread drying in formerly permafrost-affected regions—supporting the hypothesis of a permafrost-cloud feedback. Additionally, we use multiple Earth-system model simulations to quantify the temperature contribution of this feedback under a high-warming scenario. Our results show a robust global temperature increase across all model setups, driven by reduced water availability due to permafrost degradation.

How to cite: de Vrese, P., Stacke, T., Gayler, V., and Brovkin, V.: Permafrost cloud feedback, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15161, https://doi.org/10.5194/egusphere-egu26-15161, 2026.

EGU26-15197 | Orals | CR4.1

Long-term Observations of CO₂ Fluxes during the Snow-free Period in a High Arctic Dry Tundra 

Hyewon Hwang, Namyi Chae, Bang Yong Lee, Ji Young Jung, and Taejin Choi

The Arctic is undergoing rapid warming, leading to significant changes in permafrost stability and ecosystem carbon exchange. Arctic tundra ecosystems store nearly half of the world's soil carbon, yet permafrost thaw may enhance carbon dioxide emissions, amplifying climate feedbacks. Despite their importance, large uncertainties remain regarding the role of high latitude permafrost regions in the Arctic carbon cycle. The Canadian Arctic covers extensive and heterogeneous landscapes, emphasizing the need for long-term site-based observations of net ecosystem exchange (NEE). In this study, we quantify and characterize carbon dioxide fluxes during the snow-free period using the eddy covariance method at a dry tundra site in Cambridge Bay, Nunavut, Canada. The analysis is based on nine years of eddy covariance observations collected between 2012 and 2022, excluding 2020 and 2021. Carbon dioxide exchange was examined during the snow-free period from mid-June to early September, when vegetation activity plays a dominant role in ecosystem carbon dynamics. The climate at Cambridge Bay is characterized by cold and dry conditions, with a 30-year mean annual temperature of approximately −13 °C and low annual precipitation (~145 mm), typical of a dry tundra ecosystem. The site has experienced a long-term warming trend of approximately +0.0415 °C per year over the period 1953–2022. Snow cover generally persists from September to May, and snowmelt typically begins in late May to early June, marking the onset of the snow-free and biologically active period. Results show that carbon dioxide fluxes during the snow-free period are strongly influenced by vegetation growth, with peak plant productivity and maximum carbon uptake occurring during the growing season between mid-July and early August. During this period, gross primary production exceeds ecosystem respiration, resulting in net carbon uptake. On average, the growing season NEE was −40.5 g C m⁻², with corresponding gross primary production (GPP) and ecosystem respiration (Reco) of 94.2 g C m⁻² and 53.6 g C m⁻², respectively. Notably, 2017 exhibited an unusually early onset of vegetation activity, leading to enhanced carbon uptake during the snow-free period. These flux estimates highlight the important role of the dry tundra ecosystem at Cambridge Bay in the pan-Arctic carbon dioxide budget. These findings provide robust observational evidence of snow-free period carbon dynamics in a high latitude Arctic dry tundra ecosystem and improve our understanding of how ongoing climate warming may influence carbon fluxes in permafrost regions. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2025-24683148)

How to cite: Hwang, H., Chae, N., Lee, B. Y., Jung, J. Y., and Choi, T.: Long-term Observations of CO₂ Fluxes during the Snow-free Period in a High Arctic Dry Tundra, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15197, https://doi.org/10.5194/egusphere-egu26-15197, 2026.

EGU26-15489 | Posters on site | CR4.1

Characteristics of Carbon Fluxes for Tundra Ecosystems Adjacent to a Pond in Arctic Canada 

Namyi Chae, Hyewon Hwang, Taejin Choi, and Bang Yong Lee

The Arctic permafrost is a large carbon pool that is highly sensitive to climate change. Carbon fluxes were examined to understand the characteristics of the carbon cycle in tundra ecosystems adjacent to a pond. Freshwater lakes (large-scale) and ponds (small-scale) within the Arctic terrestrial ecosystem play important biogeochemical roles and, in some cases, are major sources of greenhouse gas emissions. Globally, lakes are primarily distributed in Canada and Russia, accounting for 42% and 49% of the total, respectively. The study site is located on dry tundra with a pond in the High Arctic near Cambridge Bay, Nunavut, Canada (69°7′47.7″N, 105°3′35.3″W). CO₂ and CH₄ fluxes were measured in the tundra ecosystem to evaluate the potential future sensitivity of the carbon cycle to climate change during the summers of 2019, 2022, and 2025. The vegetation cover around the site mainly consists of dwarf shrubs, graminoids, and lichens. Carbon fluxes were compared under different soil water content conditions. Based on the chamber measurements, the variability of net CO₂ exchange was more sensitive in grasses under wet conditions than in vegetation under dry conditions, and both the variability and magnitude of CH₄ emissions near ponds were greater than those under dry conditions. CO₂ and CH₄ fluxes showed a positive relationship in nearly bare soil under wet conditions and a negative relationship in areas with various vegetation under dry conditions. Net ecosystem exchange, ecosystem respiration, and gross primary production were estimated using two types of chambers to investigate the influence of carbon dynamics on the tundra carbon cycle. Carbon fluxes were compared across three years during the snow-free season, and the controlling factors of the carbon cycle were examined. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2025-24683148).

How to cite: Chae, N., Hwang, H., Choi, T., and Lee, B. Y.: Characteristics of Carbon Fluxes for Tundra Ecosystems Adjacent to a Pond in Arctic Canada, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15489, https://doi.org/10.5194/egusphere-egu26-15489, 2026.

EGU26-17019 | Posters on site | CR4.1

Soil moisture as a key control on active layer thickness prediction on James Ross Island, Antarctica 

Filip Hrbáček, Michaela Kňažková, Lucia Kaplan Pastíriková, Michael Matějka, Karolína Kohoutková, and Tomáš Uxa

Thermal properties of permafrost-affected soils play a key role in determining their response to ongoing climate warming. These properties influence the rate of active layer thickening and govern whether permafrost degradation is amplified or inhibited. Soil thermal characteristics are closely linked to other physical soil factors, with moisture often considered the most critical due to its potentially high interannual variability. In the eastern Antarctic Peninsula, projections indicate precipitation changes between −5 and +10%. However, it remains unclear whether these changes will have a noticeable effect on soil moisture, as the area is generally classified as polar-arid, with very low effective precipitation throughout the year. We therefore hypothesize that drying mechanisms will prevail, namely (a) increasing surface evapotranspiration driven by surface warming and (b) enhanced infiltration into the ground due to thickening of the active layer.

In this study, we present potential trajectories of active layer thickness (ALT) evolution on James Ross Island, Antarctic Peninsula, for the period 2010–2050 and different soil moisture scenarios. ALT was predicted using the Stefan model parameterized by: (a) climate outputs from the WRF model forced by SSP2-4.5 at a 2 km spatial resolution and (b) laboratory analysis of the relationship between soil thermal conductivity and soil moisture. Experiments were conducted using an ISOMET 2114 soil thermal properties analyzer on samples collected from three sites. Soil thermal properties were measured on samples with a fixed bulk density across several moisture states, ranging from fully saturated to completely dry.

The Stefan model was run for four soil moisture scenarios (5%, 15%, 25%, and 35%). Predicted ALT under the driest scenarios (5% and 15%) was approximately 40 cm deeper than under the wettest scenario (35%). Overall, the results indicate an increase in ALT under SSP2-4.5 conditions by 2050.

How to cite: Hrbáček, F., Kňažková, M., Kaplan Pastíriková, L., Matějka, M., Kohoutková, K., and Uxa, T.: Soil moisture as a key control on active layer thickness prediction on James Ross Island, Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17019, https://doi.org/10.5194/egusphere-egu26-17019, 2026.

EGU26-18508 | ECS | Posters on site | CR4.1

Modelling the carbon cycle in permafrost in a simplified thermal soil model coupled with iLOVECLIM  

Mathis Voisin, Aurelien Quiquet, Nathaelle Bouttes, and Didier Roche

During the Last Glacial Maximum (LGM, 21000 years ago), atmospheric CO₂ concentrations were approximately 100 ppm lower than during the pre-industrial period, yet the mechanisms responsible for this difference remain poorly understood. Several hypotheses have been proposed, involving ocean circulation, the marine biosphere, or continental carbon stocks, but none has been able to fully explain this difference. Carbon stored in permafrost soils may represent a significant and still poorly constrained component of this missing carbon reservoir.

This study investigates the role of permafrost as a long-term carbon reservoir from the LGM to the present using a modelling approach. A simple soil thermal model (FROG) is used to simulate permafrost extent, depth, active layer thickness and soil carbon content down to 1000 meters depth. The model is coupled to iLOVECLIM, an intermediate-complexity Earth System Model coupling atmosphere, ocean, and biosphere components. This approach allows transient simulations to be performed over several thousand years, which is necessary to better represent carbon cycle evolution during glacial–interglacial cycles.

Simulations are conducted for present-day and LGM climate conditions. The model produces spatially explicit estimates of permafrost extent, active layer thickness, and soil carbon distribution for both periods. Results indicate substantial differences in permafrost depth and spatial coverage between the LGM and present day. Model results are compared with available observational datasets for permafrost and soil carbon, as well as outputs from other climate models.

How to cite: Voisin, M., Quiquet, A., Bouttes, N., and Roche, D.: Modelling the carbon cycle in permafrost in a simplified thermal soil model coupled with iLOVECLIM , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18508, https://doi.org/10.5194/egusphere-egu26-18508, 2026.

EGU26-19398 | Orals | CR4.1

Estimating Vulnerable Carbon in Thawing Northern High-Latitude Permafrost Using CMIP6 Climate Projections 

Imran Nadeem, Nebojsa Nakicenovic, Asma Yaqub, Boris Sakschewski, Sina Loriani, Govindasamy Bala, Thejna Tharammal, Caroline Zimm, and Hafsa Aeman

Permafrost degradation across the Northern Hemisphere is projected to continue and intensify under ongoing climate warming, with important implications for the global carbon cycle. Thawing permafrost exposes previously frozen soil organic carbon (SOC) to microbial decomposition, resulting in the release of carbon dioxide and methane, thus potentially amplifying climate change through positive feedbacks. Robust projections of permafrost thaw are therefore essential for improving estimates of future carbon emissions and the global carbon budget.

Using output from the latest generation of global climate models participating in CMIP6, we assess changes in the annual active layer thickness (ALT), defined as the maximum seasonal thaw depth of permafrost, under four Shared Socioeconomic Pathway (SSP) scenarios (SSP1-2.6, SSP2-4.5, SSP3-7.0, and SSP5-8.5). We show that ALT estimates derived directly from CMIP6 soil temperature fields exhibit substantial deviations from observed ALT values, which can lead to inconsistent estimates of permafrost carbon release.

To address this limitation, we propose a simplified, observation-constrained approach that focuses on projected changes in ALT rather than absolute model-derived values. These projected ALT changes, combined with present-day ALT observations, are used to estimate vulnerable carbon under future climate projections. We validate our ALT-based approach through comparison with simulations from the Lund–Potsdam–Jena managed Land (LPJmL) dynamic global vegetation model, which explicitly represents permafrost and soil thermal processes. This comparison shows consistent spatial patterns of active layer thickness, supporting the robustness of our simplified estimation framework.

CMIP6 models project ALT changes of 0.1–0.3 m per degree rise in local temperature, resulting in an average deepening of approximately 1.2–2.1 m in the northern high latitudes under different scenarios. With increasing temperatures, permafrost thawing initiates in southern Siberia, northern Canada, and Alaska, and progressively extends poleward, reaching much of the Arctic under high-emissions scenarios (SSP5-8.5) by the end of the century. Using projections of ALT changes and vertically resolved SOC data, we estimate ensemble-mean decomposable carbon stocks in thawed permafrost of approximately 115 GtC under SSP1-2.6, 180 GtC under SSP2-4.5, 260 GtC under SSP3-7.0, and 300 GtC under SSP5-8.5 by 2100.

How to cite: Nadeem, I., Nakicenovic, N., Yaqub, A., Sakschewski, B., Loriani, S., Bala, G., Tharammal, T., Zimm, C., and Aeman, H.: Estimating Vulnerable Carbon in Thawing Northern High-Latitude Permafrost Using CMIP6 Climate Projections, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19398, https://doi.org/10.5194/egusphere-egu26-19398, 2026.

EGU26-22122 | Posters on site | CR4.1

Energy conservative solutions for coupled heat-mass transport in frozen soils and snow 

Andrew Ireson, Alana Muenchrath, and Chris Spence

Physically based frozen soil models are essential for understanding hydrological processes in cold regions, particularly snowmelt infiltration into seasonally frozen soils and permafrost thaw. While significant progress has been made in modeling coupled heat and mass transport in frozen soils, and several sophisticated physically based models exist, practical applications require robust coupling between snow and soil models. Although we have well-developed physically based snow models, state-of-the-art soil models are typically not integrated with them. Notable exceptions include the Cold Regions Hydrological Model (CRHM) and various land surface models such as CLASS, CLASSIC, SVS, and SUMMA. However, these models are often applied with coarse vertical resolution and, in some cases, rely on oversimplified process representations. The objective of this study is to develop a simple, point scale mass- and energy-conservative coupled snow-soil model that can be used to systematically evaluate the numerous implicit and explicit assumptions embedded in existing models. A particular focus is to evaluate various approaches for representing the upper boundary condition of the soil, which plays a critical role in governing heat and mass fluxes and, consequently, the thermal and hydrological behavior of the soil.

How to cite: Ireson, A., Muenchrath, A., and Spence, C.: Energy conservative solutions for coupled heat-mass transport in frozen soils and snow, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22122, https://doi.org/10.5194/egusphere-egu26-22122, 2026.

EGU26-1728 | ECS | PICO | CR4.2

Optimizing Electrical Resistivity Tomography Acquisition Strategies in Rock Glacier Environments 

Mirko Pavoni, Mauro Guglielmin, Jacopo Boaga, Giorgio Cassiani, Alberto Carrera, Simone Peracchi, Matteo Zumiani, Emanuele Forte, Stefano Ponti, and Luca Peruzzo

Electrical Resistivity Tomography (ERT) is a widely used geophysical method for investigating permafrost in challenging mountain environments, such as rock glaciers (Hauck and Kneisel, 2008). This study focuses on optimizing ERT acquisition strategies using modern high-quality multi-channel georesistivity meters, steel-net electrodes, and appropriate acquisition schemes, in order to efficiently and rapidly acquire multiple ERT transects and reliably characterize the internal structure of rock glaciers, despite complex surface conditions.

As recently proposed by Pavoni et al. (2025), the use of light steel-net electrodes facilitates the deployment and removal of ERT transects in blocky terrain, ensuring optimal galvanic contact without compromising data quality. In addition to these practical benefits, the choice of acquisition scheme strongly influences survey efficiency and data reliability. Hybrid acquisition schemes based on Dipole-dipole and Multigradient multi-skip approaches, when combined with multi-channel instruments, allow for rapid data acquisition, improved model sensitivity, and enhanced evaluation of dataset quality.

In this work, we compare the performance of a mixed Dipole-dipole and Multigradient multi-skip scheme with the traditional Wenner-alpha configuration. While traditional Wenner-alpha measurements are usually acquired only in the direct configuration, the Dipole-dipole and Multigradient schemes enables the acquisition of a substantially larger number of quadripoles within the same time frame, including both direct and reciprocal measurements, which provide a more robust estimation of data error by accounting for both instrumental and systematic contributions (Binley et al., 1995).

Furthermore, we evaluate the Polo-Dipole configuration’s potential to increase model sensitivity at depth (White et al., 2003), facilitating a more reliable identification of the bottom of the frozen layer within rock glaciers. Measurements were collected in both direct and reciprocal geometries, with the remote electrode deployed at two different positions and two different distances on opposite sides of the transect. Testing these alternative positions and distances of the remote electrode provided an additional way to assess data quality, confirming the robustness of the Polo-Dipole setup and its ability to increase investigation depth without significantly affecting acquisition time.

Overall, the integration of high-quality multi-channel instruments, light steel-net electrodes, and optimized acquisition strategies enhances model sensitivity and data-quality assessment while improving operational efficiency. This approach enables the rapid acquisition of multiple transects within a single field campaign and supports the development of quasi-3D resistivity models of rock glacier structures.

References

Binley, A., Ramirez, A., & Daily, W. (1995, April). Regularised image reconstruction of noisy electrical resistance tomography data. In Proceedings of the 4th Workshop of the European Concerted Action on Process Tomography, Bergen, Norway (pp. 6-8).

Hauck, C., and Kneisel, C.: Applied Geophysics in Periglacial Environments, Cambridge University Press., 2008.

Pavoni, M., Peruzzo, L., Boaga, J., Carrera, A., Barone, I., & Bast, A. (2025). Brief communication: Use of lightweight and low-cost steel net electrodes for electrical resistivity tomography (ERT) surveys performed on coarse-blocky surface environments. The Cryosphere, 19(10), 4141-4148.

White, R. M. S., Collins, S., & Loke, M. H. (2003). Resistivity and IP arrays, optimised for data collection and inversion. ASEG Extended Abstracts, 2003(2), 1-4.

How to cite: Pavoni, M., Guglielmin, M., Boaga, J., Cassiani, G., Carrera, A., Peracchi, S., Zumiani, M., Forte, E., Ponti, S., and Peruzzo, L.: Optimizing Electrical Resistivity Tomography Acquisition Strategies in Rock Glacier Environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1728, https://doi.org/10.5194/egusphere-egu26-1728, 2026.

EGU26-5157 | ECS | PICO | CR4.2

GRIT: Geospatial Rock-glacier Ice Thickness Model through Satellite-Derived Rheological Inversion 

Varun Khajuria, Shaktiman Singh, Luca Paro, Matteo Spagnolo, and Adriano Ribolini

As climate change leads to the retreat of mountain glaciers worldwide, rock glaciers are increasingly recognised as important hydrological buffers in high-altitude catchments. Unlike clean-ice glaciers, these debris-covered formations are geophysically complex, making regional estimates of their water storage consistently challenging. Current assessments usually rely on simple area–volume scaling methods based on the surface slope, which overlook the flow behaviour of individual landforms.

In this contribution, we introduce GRIT (Geospatial Rock-glacier Ice Thickness Model), an open-source computational framework that infers ice thickness from satellite-derived surface kinematics, applying a Glen-type viscous flow law. It determines thickness by integrating local slope data from a high-resolution digital elevation model (DEM) with surface horizontal velocity measurements obtained through feature tracking in high-resolution optical satellite imagery.

To constrain the rheology, we calibrate the effective creep parameter (B) using 80 MHz ground-penetrating radar (GPR) profiles collected at the Vej del Buoc rock glacier in the Maritime Alps. Our results reveal a range of B values indicative of a significantly softer effective rheology than that of clean temperate ice, consistent with the presence of interstitial unfrozen water and debris inclusions that reduce the mixture's viscosity. GRIT is designed for scalability and can be applied to regional inventories to derive spatially explicit thickness and water-equivalent maps.

To our knowledge, this is the first satellite-based, geospatial rheological inversion toolbox specifically designed for determining rock-glacier ice thickness and water-equivalent storage. By combining satellite-observed movement with site-specific geophysical calibration, GRIT offers a scalable, physically grounded method for monitoring the debris-covered cryosphere in mountain basins with limited data and for incorporating rock-glacier ice storage into regional water resource evaluations.

How to cite: Khajuria, V., Singh, S., Paro, L., Spagnolo, M., and Ribolini, A.: GRIT: Geospatial Rock-glacier Ice Thickness Model through Satellite-Derived Rheological Inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5157, https://doi.org/10.5194/egusphere-egu26-5157, 2026.

EGU26-5624 | PICO | CR4.2

Testing the integration of InSAR and optical data for rock glacier detection in a lateral valley of Valtellina (Northern Italy)  

Daniele Pisanu, Corrado Alberto Sigfrido Camera, and Roberto Sergio Azzoni

Multi-temporal InSAR techniques allow the detection of millimetric surface displacements, making them particularly suitable for monitoring slow-moving landforms, such as rock glaciers, at a regional scale. Optical data, and in particular Short-Wave Infrared (SWIR) bands, provide complementary information by enhancing the spectral response of bare debris and poorly vegetated surfaces.

This work aims to propose a workflow to recognize the presence of rock glaciers over large areas (approximately 10-100 km2) and to distinguish them from other geomorphological units through the integration of optical and interferometric data.

The approach was tested in a restricted study area (3.7 km2) in Alpe Visogno, in the municipality of Mello (SO), within a small lateral valley on the Rhaetian side of Valtellina (Northern Italy). This area hosts an atypical rock glacier due to its exposure (south) and relatively low mean altitude (2100 m a.s.l.). Such conditions make the area particularly suitable for investigating peculiar permafrost dynamics in an alpine environment.

Interferometric analysis was conducted using ascending-orbit Sentinel-1 data, covering the period from 10 May 2024 to 24 December 2024, corresponding to the snow-free season. Open-source processing tools were used to derive surface velocity maps for the area of interest. The correction of the Atmospheric Phase Screen (APS) was carried out using the Generic Atmospheric Correction Online Service (GACOS). This choice was based on a comparison of the residuals resulting from different correction approaches. The optical data came from a single Sentinel-2 image acquired during the summer period (08 August 2024) under snow-free conditions for the entire study area, reaching up to 2670 m a.s.l. This image was selected to maximize the radiometric quality and to minimize the effects of clouds and shadows. Subsequently, a specific spectral index (Debris Index) primarily derived from SWIR bands was defined. These bands are sensitive to the presence of moisture, such as that occurring in pores and fractures, and can be used to discriminate superficial layers with different textural properties. A threshold based on the 75th percentile was applied to the Debris Index to generate polygons representing the deposits. The integration of optical and interferometric data was supported by a statistical analysis, including both boxplots and clustering techniques (k-means and hierarchical Ward’s method).

The clustering identified two groups: a fast-moving cluster (average velocity of -24.4 mm yr-1) corresponding to rock glaciers, and a slow-moving cluster corresponding to simple debris deposits (average velocity of -11.1 mm yr-1). These results are strongly corroborated by field observations, confirming the effectiveness of the workflow in discriminating rock glaciers from other debris accumulations such as talus and colluvial deposits. Future developments will focus on testing the proposed workflow over larger and more heterogeneous areas to assess its robustness and transferability at local, regional, or supra-regional scales.

This study was carried out within the framework of the Italy-Switzerland Interreg VI-A project AMALPI MORE.

How to cite: Pisanu, D., Camera, C. A. S., and Azzoni, R. S.: Testing the integration of InSAR and optical data for rock glacier detection in a lateral valley of Valtellina (Northern Italy) , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5624, https://doi.org/10.5194/egusphere-egu26-5624, 2026.

EGU26-7401 | ECS | PICO | CR4.2

Using near-continuous LiDAR monitoring to quantify erosionprocesses at a rock glacier front 

Simon Ebert, Jacob Hirschberg, Raffaele Spielmann, and Jordan Aaron

Erosion at rock glacier fronts can supply sediment to adjacent torrents, which can be mobilized as damaging debris flows. Understanding the mechanisms which govern this erosion process is therefore critical for hazard management in affected areas. Previous research shows that rock glacier advance and liquid water input are the two main drivers of erosion at rock glacier fronts. However, earlier studies that calculated erosion volumes at rock glacier fronts were limited to temporal resolutions ranging from months to years. Therefore, these studies exhibit a high uncertainty due to the opposing influences of rock glacier front advance and retrogressive erosion. This prevented an in-depth understanding of the underlying drivers of these processes and their magnitudes on a short timescale. To overcome this limitation, we adapt the setup by Aaron et al. (2023) and use a permanently installed LiDAR sensor to monitor surface changes at a rock glacier front. By calculating Digital Elevation Models of Difference (DoDs) with respect to the local surface normal, we are able to compute erosion volumes at an hourly temporal resolution. This enables the quantification of short-term and small-scale geomorphic changes at the rock glacier front, which could not be detected by previous studies.

Our study site is the fast-moving Ritigraben rock glacier (front velocity > 1cm/day) in the Mattertal (Valais). Its front is directly connected to a torrential channel, which regularly produced debris flows in the past and has been monitored for more than 30 years. Preliminary results show a link between erosion events and short-term precipitation with camera images showing signs of surface runoff in the affected areas. However, erosive events are triggered by comparatively common rainfall events. Small-scale reworking of material at the rock glacier front also occurs completely independently of precipitation events in some cases. Further investigation is needed to determine if the release of material is due to failure disposition from prior events and the rock glacier creep, or the influence of meltwater from the rock glacier body.

 

References

Aaron, Jordan, Raffaele Spielmann, Brian W. McArdell, and Christoph Graf (2023). “High-Frequency 3D LiDAR Measurements of a Debris Flow: A Novel Method to Investigate the Dynamics of Full-Scale Events in the Field”. In: Geophysical Research Letters 50.5. doi: 10.1029/2022GL102373.

How to cite: Ebert, S., Hirschberg, J., Spielmann, R., and Aaron, J.: Using near-continuous LiDAR monitoring to quantify erosionprocesses at a rock glacier front, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7401, https://doi.org/10.5194/egusphere-egu26-7401, 2026.

EGU26-8432 | ECS | PICO | CR4.2

Millennial-Scale Fire and Vegetation Change from a Rare Mid-Latitude Permafrost Fen (Beartooth Plateau, WY, USA) 

Anica Tipkemper-Wolfe, David McWethy, and Mio Alt

Long-term fire histories are well documented across most North American temperate forest systems, yet the fire regimes of high-alpine treeline environments remain poorly understood. Here, we present a millennial-scale fire history from the Sawtooth Fen Palsa (SFP), a rare permafrost fen palsa located in the high-alpine treeline ecotone of the Beartooth Plateau, Wyoming, a permafrost system now unraveling due to recent decades of rapid warming. Analysis of paleoenvironmental proxies from peat sediments overlying permafrost reveals that a multi-century peak in fire activity occurred around 10,000 cal yr BP, coinciding with the afforestation of newly deglaciated, ice-free sites. This initial surge in fire activity was followed by a decline when orbitally driven increased growing-season temperatures likely promoted forest expansion at high elevations where moisture was not limiting. High severity fire activity increased again during the mid- Holocene (approximately 6,700–5,000 cal yr BP), when effective moisture increased, favoring subalpine forest expansion and increased connectivity of woody biomass (sagebrush and forest), enhancing the potential for canopy fire spread. Generally cooler and wetter conditions and possible year-round coverage of the fen palsa with snow and ice drove a near-absence of woody biomass burning at 5,000 cal yr BP. Rapid warming in recent decades has triggered the formation of dozens of thermal collapse ponds across the fen palsa. The frequency of these features has more than doubled since 2000 AD, underscoring the degradation of underlying permafrost in response to changing climatic conditions. Continued warming is expected to cause the complete loss of the permafrost lens, with far-reaching implications for ecosystem dynamics, disturbance regimes, and carbon and nutrient cycling.

How to cite: Tipkemper-Wolfe, A., McWethy, D., and Alt, M.: Millennial-Scale Fire and Vegetation Change from a Rare Mid-Latitude Permafrost Fen (Beartooth Plateau, WY, USA), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8432, https://doi.org/10.5194/egusphere-egu26-8432, 2026.

EGU26-8973 | ECS | PICO | CR4.2

Fiber-Optic Seismology Reveals Structural–Hydrothermal Coupling in Permafrost Degradation on the Qinghai–Tibet Plateau 

Wenying Cen, Feng Cheng, Jianghai Xia, Jianbo Guan, Haoyuan Sun, Ke Zhao, Ruijie Wu, Jie Chen, and Tonghua Wu

Permafrost degradation along the Qinghai–Tibet Engineering Corridor (QTEC) poses severe risks to infrastructure stability. While current monitoring techniques often lack sufficient spatial continuity or depth resolution, Distributed Acoustic Sensing (DAS) offers a scalable alternative for subsurface characterization. This study introduces a high-resolution imaging framework that leverages existing fiber-optic infrastructure and a Convolutional Neural Network (CNN) to isolate transient traffic-induced vibrations from low Signal-to-Noise Ratio (SNR) DAS records. By selectively stacking these detected signals, we expand the recoverable frequency range of ambient noise interferometry to 45 Hz (vs. 35 Hz for standard stacking), enabling the reconstruction of a 2D shear-wave velocity (Vs) profile near the Kunlun Mountain Pass. The imaging results clearly delineate the permafrost table and base, revealing a permafrost thickness of up to 90 m. Furthermore, we identify pronounced lateral heterogeneities and a structural discontinuity interpreted as a fault-controlled talik. This subsurface anomaly spatially coincides with localized subsidence observed via InSAR, highlighting a coupled structural–hydrothermal mechanism for degradation. Our workflow demonstrates the efficacy of AI-enhanced "dark fiber" sensing for identifying concealed cryospheric hazards in remote alpine regions.

 

How to cite: Cen, W., Cheng, F., Xia, J., Guan, J., Sun, H., Zhao, K., Wu, R., Chen, J., and Wu, T.: Fiber-Optic Seismology Reveals Structural–Hydrothermal Coupling in Permafrost Degradation on the Qinghai–Tibet Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8973, https://doi.org/10.5194/egusphere-egu26-8973, 2026.

Permafrost mapping in high-mountain environments is essential for understanding cryospheric processes and assessing cryopheric hazards due to climate change. Remote sensing-based permafrost mapping commonly relies on multiple climatological and topographical parameters, including land surface temperature, snow index, soil moisture, elevation, slope and aspect. However, accurately predicting subsurface permafrost conditions remains challenging.  For mountain permafrost studies, rock glaciers are widely used as proxies for permafrost presence, and machine-learning models are often trained primarily on their spatial distribution. This approach introduces a systematic bias, as rock glaciers are typically concentrated above ~4200 m a.s.l., whereas permafrost occurrence is also controlled by local thermal regimes, soil properties, and moisture conditions, allowing its presence within valley settings. In this study, we investigate mountain permafrost occurrence and active layer characteristics in contrasting high-altitude environments using an integrated remote sensing and geophysical approach. Ground Penetrating Radar (GPR) surveys were carried out at two different geographical locations, Matiyan, Jammu and Kashmir, and Baralachala, Himachal Pradesh. The locations were chosen for their diverse lithology, elevation and climatic conditions. GPR data was collected in both common-offset and multi-offset modes using 80 MHz and 450 MHz antennas, aiming to enhance depth and resolution. The GPR data reveal clear subsurface signatures of frozen ground, including ice-rich layers and distinct active layer thicknesses, even in areas lacking visible rock glacier morphology. The ALT measurements ranged from 0.6 m to 1.2 meters depth in Matiyan, while Baralachala showing a shallower active layer of 0.2 m to 0.5 meters and reflecting colder climatic conditions and less surface disturbance. The findings of this study highlight the limitations of proxy-based permafrost mapping and provide a deeper understanding of mountain permafrost in changing climatic scenarios. Thus, the integration of remote sensing data with subsurface observations provides improved understanding of thermo-hydrological controls on mountain permafrost distribution.

How to cite: Mahanta, K. K. and Shukla, D. P.: Integrating Geophysical and Remote Sensing Techniques for Mountain Permafrost mapping in the Northwestern Himalaya, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10206, https://doi.org/10.5194/egusphere-egu26-10206, 2026.

EGU26-11138 | ECS | PICO | CR4.2

The role of permafrost in large rock slope failures in the early Holocene - An analysis of the Köfels rock slide (3.1 billion m³) 

Felix Pfluger, Lily Bever, Samuel Weber, Johannes Fürst, and Michael Krautblatter

Some of the largest rock slope failures in the European Alps today occurred with a significant lag time of several thousand years after glaciers retreated from the Last Glacial Maximum. Amongst other processes, the inert permafrost evolution can partly explain the delayed failure timing. Here, we challenge this hypothesis using the Köfels rock slide (Austria, 3.1 km³ failure volume, 9527–9498 cal BP) by retracing thermal conditions and reassessing the failure mechanics of one of the most prominent crystalline rock slides in the Alps. Our coupled simulations of ice-permafrost temperatures suggest that permafrost was maintained at the upper slope parts, mainly above glacier surface elevations, throughout the past 40 ka. Yet in the period before the rock slope failure, permafrost was preserved only at the highest elevation. It was lost within the hanging valley behind the failed mountain flank. This likely led to hydrogeological recoupling, enhancing groundwater flow towards stability-relevant zones. In addition, we deploy new rock mechanical tests to assess the rock bridge shear strength of the local orthogneiss and run mechanical simulations in order to decipher and better discuss the complex promoting factors of the Köfels rock slide (currently in process). Large permafrost rock slope failures are not only attributed to the loss of cohesive rock and ice material strength by warming temperatures, rather than to the interwoven hydro-thermo-mechanical system adaptation resulting from permafrost degradation.

How to cite: Pfluger, F., Bever, L., Weber, S., Fürst, J., and Krautblatter, M.: The role of permafrost in large rock slope failures in the early Holocene - An analysis of the Köfels rock slide (3.1 billion m³), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11138, https://doi.org/10.5194/egusphere-egu26-11138, 2026.

EGU26-13607 | ECS | PICO | CR4.2

Long-term Passive Seismic Monitoring of Permafrost Dynamics at the Matterhorn Hörnligrat (Valais, Switzerland) 

Valeria Strallo, Chiara Colombero, Jan Beutel, and Samuel Weber

Permafrost degradation in alpine regions driven by climate warming is increasing the likelihood of rock slope destabilization. However, the mechanical response of fractured rock-ice systems to repeated freeze-thaw cycles and long-term warming remains poorly monitored and understood. Using a decade of continuous passive seismic data recorded at different stations, this study investigates how seasonal and long-term environmental forcings affect the mechanical properties of a steep bedrock permafrost site at the Matterhorn Hörnligrat ridge (Valais, Switzerland). We applied spectral analysis (single-station and site-reference spectral ratios), auto- and cross-correlation of ambient seismic noise combined with microseismic event detection and analysis to track the long-term temporal variations and evolution in resonance frequencies and seismic wave velocity within the rock mass, and in the spectral characteristics of microfracturing events. We observed strong, reversible seasonal variations of mechanical parameters linked to freeze-thaw cycles, characterized by reduced stiffness in summer and increased stiffness in winter. Long-term observations showed a continuous decrease in resonance frequencies, wave velocities, and peak frequencies of the microseismic events, indicating progressive and irreversible mechanical weakening of the rock-ice system. 
These results demonstrate that passive seismic monitoring enables the detection of both reversible and irreversible mechanical changes in alpine permafrost slopes, providing early indicators of progressive destabilization under ongoing climate warming.

How to cite: Strallo, V., Colombero, C., Beutel, J., and Weber, S.: Long-term Passive Seismic Monitoring of Permafrost Dynamics at the Matterhorn Hörnligrat (Valais, Switzerland), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13607, https://doi.org/10.5194/egusphere-egu26-13607, 2026.

EGU26-14051 | ECS | PICO | CR4.2

Advancement in Permafrost Modeling: The Role of Adsorption-Aware Thermodynamics in Fine-Grained Soils 

Marianna Tavonatti, John Mohd Wani, Stephan Gruber, and Riccardo Rigon

Permafrost and seasonally frozen ground are critical components of the Arctic cryosphere, playing a fundamental role in regulating hydrological processes. Permafrost underlies approximately 13-18% of the Northern Hemisphere’s exposed land surface and stores vast quantities of organic carbon. Its thermal stability has profound implications for infrastructure, carbon cycle, and hydrological processes under changing climate. Modeling permafrost dynamics is critical, yet standard cryo-hydrological models often struggle to capture the complex phase changes in fine-grained soils, particularly in clayey soils where liquid water persists at temperatures well below the classical freezing point.

To overcome this challenge, we propose an advanced thermodynamic framework that moves beyond the classical soil freezing characteristic curves (SFCC). By incorporating adsorption potential (μads), this framework accounts for the exponential energy decay near mineral surfaces, physically explaining the persistence of liquid water in clay nanopores down to −80℃. While the theoretical foundation for this approach is established in the enthalpy-based solver WHETGEO-1D (Tubini & Rigon, 2022), we evaluate its significance through a comparative study using field forcing and hypothetical experiments.

We conducted this analysis in two stages. First, the 1D GEOtop model was applied to two sites along the Inuvik-Tuktoyaktuk Highway (Canada) using ERA5 and JRA-3QG reanalysis data (1950–2023). At this stage, the model performance was evaluated against ground temperature observations (2017–2022) to ensure realistic surface fluxes and ground temperatures. Second, using these validated forcing conditions, we performed hypothetical experiments to compare the classical and adsorption-aware frameworks across different soil types.

Our initial analysis indicates that the classical and adsorption-aware frameworks yield divergent results in the timing of latent heat exchange and moisture redistribution. By bridging the gap between pore-scale thermodynamics and Darcy-scale modeling, this study provides a robust roadmap for implementing next-generation physics into permafrost models.

How to cite: Tavonatti, M., Wani, J. M., Gruber, S., and Rigon, R.: Advancement in Permafrost Modeling: The Role of Adsorption-Aware Thermodynamics in Fine-Grained Soils, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14051, https://doi.org/10.5194/egusphere-egu26-14051, 2026.

EGU26-14080 | ECS | PICO | CR4.2

Understanding the low-frequency electrical properties of ice–water interfaces from laboratory and field experiments 

Clemens Moser, Alexander Bast, Sophie Marie Francis, Matthias Halisch, Christian Hauck, and Adrián Flores Orozco

Quantifying ice and water in the subsurface is key to advancing our understanding of permafrost-related processes and to supporting hydrogeological management in cold regions. Electrical resistivity methods are well established as non-invasive tools for discriminating between frozen and unfrozen ground due to the high resistivity of frozen materials. However, solid rocks are also highly resistive, which makes a quantitative estimation of ice content based on resistivity alone challenging. The spectral induced polarization (SIP) method, which allows to measure the conductivity and polarization of rocks and soils, has been proposed as a complementary method for the investigation of frozen ground as ice exhibits a characteristic polarization response in the kHz frequency range due to protonic defects in its crystal lattice. In practice, however, collecting SIP data in such a frequency range is challenging, particularly in alpine environments, due to the logistical constraints and strong capacitive coupling effects related to the high contact resistance between electrodes and the ground. Recently, polarization effects at lower frequencies (< 100 Hz) associated with ice–water interfaces have been reported at the field scale and in laboratory experiments. To quantitatively assess these effects, we present results from experiments conducted at two different scales. First, we show laboratory experiments investigating the SIP response of blank ice features in solid rocks with varying ice volumes and temperatures ranging from +5 °C to −10 °C. Second, we present field SIP data collected during summer 2025 using borehole electrodes in the active rock glacier Muragl (Grisons, Swiss Alps). In the laboratory experiments, holes were drilled into rock samples and SIP measurements were performed after filling the holes with air, water, or ice, allowing a direct comparison of the polarization response for the different pore fillings. We identify a strong polarization effect below 100 Hz for ice-filled holes, while the response remains low when the holes are filled with water or air. Increasing the hole size—and thus the ice volume and the ice–water–rock interfacial area—results in an increase in the polarization strength and a shift of the maximum polarization toward lower frequencies. The SIP field data were acquired using borehole tomography, as borehole electrodes are positioned closer to the ground ice than surface electrodes, enabling a more direct comparison between field and laboratory observations. The results reveal an anomaly characterized by low electrical conductivity and increased polarization starting at approximately 1 Hz in a depth where drillings in summer 2024 revealed relatively high ice content. Overall, our results confirm the presence of a low-frequency polarization effect at ice–water interfaces and demonstrate its potential to image ground ice in alpine permafrost and seasonally frozen soils.

How to cite: Moser, C., Bast, A., Francis, S. M., Halisch, M., Hauck, C., and Flores Orozco, A.: Understanding the low-frequency electrical properties of ice–water interfaces from laboratory and field experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14080, https://doi.org/10.5194/egusphere-egu26-14080, 2026.

Due to climate change, ice masses are thawing rapidly. This leads to drastic changes in water discharge, increased erosion, decreased biodiversity, as well as an increasing risk of droughts. However, the amount of subsurface ice is often unknown. To better understand the implications of decreasing ice masses, the first step is to determine the initial ice distribution of the region of interest. One of the few places in the German Alps where we still find glaciers and permafrost is the Zugspitze. It is the highest mountain in Germany and has a long observational history dating back to 1820, which is present-day coordinated by the Virtual Alpine Observatory.

Here, we present the framework of creating a complement first dataset by conducting electrical resistivity tomography measurements and seismic refraction tomography. For this, we will measure ca. ten profiles across the 2 km diameter of the horseshoe-shaped Zugspitzplatt to decipher permafrost ice contents within the blocky surface, ice depth distribution and its state of degradation. To verify those findings, the model is tested against both data from a superconductive gravimeter and the isotopic concentration of the outflow to distinguish glacier water from permafrost water. This contribution shows the conceptual framework with which we will analyze the future water potential coming from the permafrost at the Zugspitzplatt in the framework of the AlpSenseAdapt project.

How to cite: Gahr, S. and Krautblatter, M.: Using electrical resistivity tomography and seismic refraction tomography to decipher permafrost ice distribution and loss at the Zugspitze (Germany) complementary to superconductive gravimeter and isotope chemistry measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18413, https://doi.org/10.5194/egusphere-egu26-18413, 2026.

EGU26-20454 | ECS | PICO | CR4.2

PermaCOST: New International Research Network for Coordinated and Standardised Monitoring of Permafrost Response to Climate Change 

Coline Mollaret, Filip Hrbacek, Line Rouyet, Ylva Sjöberg, Flavius Sirbu, Mohammad Farzamian, Jan Blöthe, Francesco Brardinoni, Cécile Pellet, Andreas Kellerer-Pirklbauer, Manja Zebre, and Alina Milceva

PermaCOST is a new international research network funded by the COST Action Association of the European Union (CA24157). This four-years project (2025-2029) brings together European permafrost researchers, stakeholders, and practitioners with expertise in different measurement techniques and permafrost conditions to work towards a coordinated and standardised monitoring of permafrost response to climate change.

Permafrost has been dramatically warming and degrading in most mountain and polar regions, with far-reaching and long-term implications for natural and anthropogenic environments. In this context of rapid changes and large socio-economic impacts, the increased scrutiny from the society and the growing demand for sound data from stakeholders make permafrost monitoring a timely and highly relevant field of research.

Documenting, analysing, and assessing the response of permafrost to climate change requires fundamental cross-disciplinary and cross-geographic knowledge that can only be achieved through coordinated and standardized monitoring activities. For years, European research groups have been at the forefront of operational and innovative permafrost monitoring activities, but they have not been able to further coordinate their activities or to establish widely accepted standards for data acquisition and processing.

Through an unprecedented network of experts and early career investigators, PermaCOST aims to promote and foster operational networking of permafrost researchers, stakeholders and practitioners to facilitate an overall comparability of data sets and time series of various permafrost variables for a better characterisation of the long-term permafrost evolution on the global scale.

PermaCOST is organised in five Working Groups (WGs) with the specific objectives to identify key novel permafrost monitoring methods (WG1), to homogenise permafrost data acquisition standards (WG2) and permafrost data processing standards (WG3), to assess the state and evolution of permafrost in Europe (WG4) and to promote the development of operational permafrost monitoring networks at national, regional, and European scales (WG5).

In this contribution, we will present the objectives and structure of the project, as well as the concrete tasks and ongoing activities in the WGs covering mountain, polar and marginal permafrost. We will also inform the permafrost community on how to join the network, and take advantage of the upcoming opportunities for networking, training, and research collaboration, through short-term scientific missions, travel grants, training schools and workshops.

How to cite: Mollaret, C., Hrbacek, F., Rouyet, L., Sjöberg, Y., Sirbu, F., Farzamian, M., Blöthe, J., Brardinoni, F., Pellet, C., Kellerer-Pirklbauer, A., Zebre, M., and Milceva, A.: PermaCOST: New International Research Network for Coordinated and Standardised Monitoring of Permafrost Response to Climate Change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20454, https://doi.org/10.5194/egusphere-egu26-20454, 2026.

EGU26-20730 * | ECS | PICO | CR4.2 | Highlight

Impact of permafrost changes on the 2025 Nesthorn-Birchgletscher hazard cascade 

Mylène Jacquemart, Julien Brondex, Friedrich Knuth, Samuel Weber, Robert Kenner, Jordan Aaron, Valentin Gischig, Radhika de Silva, Raffaele Spielmann, Marius Schneider, Dominik I. Schumacher, Ethan Welty, Fabian Reist, Ingrid Senn, and Daniel Farinotti

In late May 2025, a series of large rock failures from Kleines Nesthorn in the Swiss Lötschental (Lötschen valley) fell directly onto the Birchgletscher (Birch Glacier), loading the latter with around 4 million m3 of rock. On May 28, following several days of acceleration, Birchgletscher collapsed in its entirety, claiming one life and causing the near-total destruction of the historic village of Blatten (which had been fully evacuated prior to the event). Totaling more than 9 million m3 of rock and glacier ice (with a ratio of about 3:1), the rock-ice avalanche dammed the river Lonza and led to the formation of a lake that damaged additional parts of the village.

The rock failures that initiated the hazard cascade originated from the north-east face of Kleines Nesthorn, a formerly 3336 meter tall peak. Like all areas at this elevation, this face is expected to have experienced important ground temperature changes in the past decades. In this contribution, we ask how these changes may have affected the observed hazard cascade. We analyzed climatic changes (air temperature and precipitation) and snow cover, simulated permafrost changes, and assessed the geologic preconditioning and failure kinematics. We then attempt to propagate these changes through the hazard cascade to understand their possible impact on the rock slope failures. To do so, we employed a combination of data from weather stations, satellite data, climate models and numerical modeling. Our findings demonstrate the complexity of the Nesthorn-Birchgletscher hazard cascade and highlight challenges and research gaps for assessing the role of permafrost on large rock slope failures in a changing climate.

How to cite: Jacquemart, M., Brondex, J., Knuth, F., Weber, S., Kenner, R., Aaron, J., Gischig, V., de Silva, R., Spielmann, R., Schneider, M., Schumacher, D. I., Welty, E., Reist, F., Senn, I., and Farinotti, D.: Impact of permafrost changes on the 2025 Nesthorn-Birchgletscher hazard cascade, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20730, https://doi.org/10.5194/egusphere-egu26-20730, 2026.

This paper discusses mechanical modelling strategies for instable permafrost bedrock. Modelling instable permafrost bedrock is a key requirement to anticipate magnitudes and frequency of rock slope failures in a changing climate but also to forecast the stability of high-alpine infrastructure throughout its lifetime.  

The last 5-10 years have brought upon significant advances in the (i) knowledge of relevant hydrostatic pressures in permafrost rock, (ii) the brittle-ductile transitions of ice relevant for larger permafrost rock slope failures and (iii) techniques that can help to decipher the preparation phase of large rockslides also (iv) many new examples have delivered additional insight into multi-phase failure.

Degrading permafrost will act to alter (i) rock mechanical properties such as compressive and tensile strength, fracture toughness and most likely rock friction, (ii) warming subcero conditions will weaken ice and rock-ice interfaces and (iii) increased cryo- and (iv) hydrostatic pressures are expected. This paper presents data and strategies how to obtain relevant (i) rock mechanical parameters (compressive and tensile strength and fracture toughness, lab), (ii) ice- and rock-ice interface mechanical parameters (lab), (iii) cryostatic forces in low-porosity alpine bedrock (lab and field) and (iv) hydrostatic forces in perched water-filled fractures above permafrost (field).

This contribution will focus on three recent events, the Bliggspitze 2007, the Fluchthorn 2023 and Kleines Nesthorn/Blatten 2025 rock slope failures which have provided significant new insights in the mechanics of premafrost rock slope detachment, due to novel observational data, lab results and resulting mechanical models. 

How to cite: Krautblatter, M., Pfluger, F., Mühlbauer, S., and Offer, M.: Understanding the mechanical destabilization of large permafrost rock slope failures using data, samples and models from the Bliggspitze 2007, Fluchthorn 2023 and Kleines Nesthorn/Blatten 2025 failures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20970, https://doi.org/10.5194/egusphere-egu26-20970, 2026.

EGU26-1097 | ECS | Posters on site | CR4.5

Echoes from the ice: assessing the effectiveness of coastal defences on underlying permafrost 

Luke Macpherson, Craig Warren, James Martin, and Mike Lim

The Hamlet of Tuktoyaktuk in the Canadian Arctic faces forced relocation due to accelerating ground ice thaw and coastal erosion, a crisis that could create Canada’s first climate refugees. The stability of the massive ground ice beneath Tuktoyaktuk Island’s newly installed shoreline defences is a critical unknown and could impact the landscape and sensitive harbour ecosystem for years to come. Our research answers the scientific question: how effective is modern climate adaptation infrastructure on the permafrost it is designed to protect?

Our expeditions will pioneer a novel, community-focused methodology to address this urgent problem, moving beyond traditional intrusive surveys. In August 2025, we conducted a pilot study to confirm the viability of our geophysical methods. In March 2026, we will conduct the first comprehensive Ground Penetrating Radar (GPR) surveys in Tuktoyaktuk since the defences were built. In partnership with the community, we will deploy the GPR from a snowmobile and venture onto the sea ice, to create high-resolution 3D maps of massive ground ice, identify areas of weakness, and track thaw by comparing our findings to a six-year historical dataset. Using new interactive tools in GPR enabling in situ processing and time-lapsing, we will develop our findings into a community-scale hazard map for the Hamlet Council which will inform adaptation and land use planning.

How to cite: Macpherson, L., Warren, C., Martin, J., and Lim, M.: Echoes from the ice: assessing the effectiveness of coastal defences on underlying permafrost, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1097, https://doi.org/10.5194/egusphere-egu26-1097, 2026.

EGU26-9055 | Orals | CR4.5

A decade of land surface deformation monitoring across Arctic lowland permafrost regions with Sentinel-1 

Annett Bartsch, Barbara Widhalm, Sree Ram Radha Krishnan, and Zhijun Liu

Ground temperatures are steadily increasing across the Arctic. Observations also show increasing active layer thickness. This leads to melt of ice at the upper permafrost boundary and changes in microtopography. Land surface deformation derived from SAR interferometry can serve as an indication for potential permafrost degradation and as a tool to describe wet/dry gradients. Progress has been made specifically with the launch of the Copernicus Sentinel-1 mission in 2014. Challenges remain including data gaps due to acquisition strategies, and ionospheric and atmospheric effects.

Sentinel-1 data availability and processing constrains have been investigated across Arctic permafrost lowlands. Specifically, the impact of spatial filtering for the reduction of ionospheric and atmospheric effects has been assessed. Within season and multiannual deformation has been derived for five distinct environments across Northern America and Northern Eurasia. Results were assessed to a range of environmental parameters including land cover and permafrost properties (Permafrost CCI records) using Random Forest regressor analyses.

On average data from half of the years could be utilized. Differences in deformation patterns were found due to region specific disturbances, but in general linkages with landcover and permafrost properties were similar across the Arctic.

How to cite: Bartsch, A., Widhalm, B., Radha Krishnan, S. R., and Liu, Z.: A decade of land surface deformation monitoring across Arctic lowland permafrost regions with Sentinel-1, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9055, https://doi.org/10.5194/egusphere-egu26-9055, 2026.

As a primary driver of anthropogenic disturbance, roads significantly impact the fragile ecological balance and serve as a critical indicator for quantifying human expansion in the Arctic wilderness. However, current geospatial datasets in these high-latitude regions suffer from severe fragmentation and limited coverage, creating a blind spot that impedes precise environmental monitoring and sustainable development planning. To address these deficiencies, this study explores the potential of utilizing Google Satellite Embeddings combined with deep learning methods to extract roads in the Arctic wilderness. Specifically, we propose the Wilderness Area Road Extraction Network (WARE-Net), a novel road extraction model based on a U-shaped architecture. The model integrates an encoder adapted for these Embeddings to enhance feature representation. To identify road morphological characteristics, a Linear Feature Enhancement Module is developed to effectively capture multi-directional linear features. Furthermore, in the decoding phase, a detection head fusing the outputs of three decoding modules is designed to improve road extraction performance. Experimental results demonstrate that WARE-Net achieves satisfactory performance on the test set, with an F1 score of 76.17% and an IoU of 63.58%. Moreover, road extraction experiments conducted in the Khanty-Mansiysky District (Russia, covering 46,400 km2) further validate the effectiveness and generalization capability of the proposed method. In conclusion, our approach holds significant promise for achieving large-scale, rapid, and accurate wilderness road extraction, thereby providing vital technical support for sustainable development assessment in the Arctic.

How to cite: Wang, J. and Liu, C.: WARE-Net: A Deep Learning Framework for Arctic Wilderness Road Extraction Using Google Satellite Embeddings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9401, https://doi.org/10.5194/egusphere-egu26-9401, 2026.

EGU26-10543 | ECS | Posters on site | CR4.5

Stochastic Modeling of Permafrost Ground Deformation Based on High-resolution InSAR Data 

Zhijun Liu, Barbara Widhalm, Annett Bartsch, Thomas Kleinen, and Victor Brovkin

Permafrost ground deformation is a disturbance process with high spatial heterogeneity. With the advent of InSAR (Interferometric Synthetic Aperture Radar) monitoring of permafrost ground deformation at meter scale, statistical approaches are becoming crucial for revealing characteristics hidden in large datasets.

For this study, we use ALOS PALSAR-2 data, covering four regions and at least three years each: Central North Slope, Mackenzie River Delta, Noatak River Basin and Yamal. Building on the approach from our previous study, we represent all meter-scale deformation data in km-scale grids using data distributions. The variance of cumulative annual permafrost ground deformation shows an approximately linear relationship with the number of years in all regions. Based on this linearity, we establish a simple stochastic model for permafrost ground deformation. With this conceptual model, the probability of a region reaching a given threshold (cm) of subsidence within a specified number of years can be derived.

We calculate Pearson correlation coefficients between ERA climate forcings and statistical moments of the ground-deformation distributions at 10 km resolution. Climatic and topographic factors at 10 km show substantially higher correlations with deformation variance and kurtosis than with mean deformation. We hypothesize that climatic impacts influence permafrost ground deformation not primarily deterministically, but through the volatility term of the stochastic process.

In addition, we quantify the intrinsic temporal memory of permafrost ground deformation using an ensemble approach.  Due to the limited time-series length, we calculate the lag-1 and lag-2 correlation coefficients by treating deformation data within the same environment condition as an ensemble in a fixed state.

This study demonstrates statistical features present in meter-scale InSAR data. Our results highlight the perspective of treating permafrost ground deformation as a stochastic process and demonstrate a potential pathway for linking km-scale climate forcings to meter-scale permafrost disturbances.

How to cite: Liu, Z., Widhalm, B., Bartsch, A., Kleinen, T., and Brovkin, V.: Stochastic Modeling of Permafrost Ground Deformation Based on High-resolution InSAR Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10543, https://doi.org/10.5194/egusphere-egu26-10543, 2026.

EGU26-12792 | ECS | Posters on site | CR4.5

Investigating Permafrost Aggradation below a Cascading Arctic Lake Drainage using Transient Electromagnetics and Thermal Modeling 

Aidan Armstrong, Rodrigo Correa Rangel, Benjamin Jones, Andrew Parsekian, Mikhail Kanevskiy, and Melissa Ward Jones

            The Arctic is warming at four times the rate of the global average which threatens the existence of permafrost. Independent of anthropogenic climate change, both degradation and aggradation of permafrost in the Arctic frequently occurs below lake and drained lake basin (L-DLB) systems. If global climate change continues at the current rate, we expect that permafrost degradation would accelerate during the extant lake phase, and that permafrost aggradation would slow and even cease if mean air temperatures begin to approach or exceed 0⁰C. Also, L-DLB systems are ubiquitous in Arctic permafrost regions, occupying between 20 - 33% of the total land of the northern circumpolar permafrost region with some areas, like the Arctic Coastal Plain of Alaska (ACPA), exceeding 80% coverage. Therefore, it is vital to study L-DLB systems to understand the dynamics of permafrost regimes in the context of a warming climate. Currently, there are limited studies that have measured permafrost dynamics below L-DLBs, almost no studies have measured aggradation immediately after lake drainage, and to our knowledge there are no designated sites to monitor aggradation rates under naturally occurring DLBs. In 2020, we were informed by local and traditional knowledge experts from Utqiagvik that a lake drainage event was likely to occur at the Bugeye Lakes Complex in the ACPA. Over the next two years, we closely observed a cascade lake drainage event that partially or completely drained all four Bugeye Lakes. This was the first time a naturally occurring cascade drainage event has been captured in real time which has provided a unique opportunity to establish a monitoring site for permafrost aggradation. To estimate talik thicknesses and aggradation rates after lake drainage, we have acquired transient electromagnetic (TEM) measurements at Bugeye Lakes in April 2022 and will repeat TEM measurements in April 2026. We have also used transient thermal models to compare with our geophysical observations. Additionally, we expect that our work will provide a framework for establishing a L-DLB monitoring site at the Bugeye Lakes Complex, which would be critical to improve our understanding of permafrost dynamics under a warmer climate regime.

How to cite: Armstrong, A., Rangel, R. C., Jones, B., Parsekian, A., Kanevskiy, M., and Ward Jones, M.: Investigating Permafrost Aggradation below a Cascading Arctic Lake Drainage using Transient Electromagnetics and Thermal Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12792, https://doi.org/10.5194/egusphere-egu26-12792, 2026.

EGU26-13504 | ECS | Posters on site | CR4.5

Assessment of an InSAR based soil moisture index across Arctic permafrost regions. 

Sree Ram Radha Krishnan, Annett Bartsch, and Barbara Widhalm

Identifying soil moisture in permafrost regions is crucial for various applications, yet it remains challenging with standard remote sensing techniques due to the high heterogeneity of the landscape. Soil wetness plays a significant role in these regions, facilitating processes such as the upscaling of carbon fluxes. Seasonal thawing and freezing of near-surface soil, in the presence of ice, cause subsidence-heave cycles with magnitudes reaching centimeters.

A recent study with focus on central Yamal showed that Sentinel-1 InSAR detects pronounced subsidence in areas with higher soil moisture using the relationship between thawing degree days and surface deformation. In this study, we extended the analysis to multiple site-specific study areas across the entire Arctic, and its performance is evaluated against other commonly used remote sensing global soil moisture products (CCI, SMAP, SMOS), reanalysis (ERA5) and in-situ measurements. Soil moisture data from various field campaigns were compiled via data mining for this purpose. Furthermore, a landscape-scale analysis is conducted to quantify biases across various terrain types and to identify wetness gradients across the study sites.

It can be demonstrated that the InSAR approach offers a valuable tool for distinguishing wet and dry landscape features, which is significant for monitoring permafrost degradation in Arctic lowland regions.

How to cite: Radha Krishnan, S. R., Bartsch, A., and Widhalm, B.: Assessment of an InSAR based soil moisture index across Arctic permafrost regions., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13504, https://doi.org/10.5194/egusphere-egu26-13504, 2026.

EGU26-13537 | Posters on site | CR4.5

Q-Arctic: synergetic observations and modeling of pan-Arctic interactions between hydrology, disturbance and carbon cycle processes 

Mathias Göckede, Annett Bartsch, Victor Brovkin, and Martin Heimann and the Q-Arctic Team

Arctic permafrost has been identified as a critical element in the global climate system, since it stores a vast amount of carbon that is at high risk of being released under climate change. The feedbacks between permafrost carbon and climate change are moderated by complex interactions between physical, hydrological, biogeochemical, and ecological processes. Many of these are not well understood to date, and therefore also only rudimentarily represented in current Earth System Models (ESMs).

The Q-ARCTIC project funded by the European Research Council (ERC) follows a synergetic approach by combining remote sensing and local-scale observations with modeling on scales from a few meters to hundreds of kilometers. The primary objective of Q-ARCTIC is to close the gap between process scales and the much coarser grid resolution of Earth System Models (ESMs), with a particular focus on the net effect of disturbance processes and associated changes in hydrology on the pan-Arctic scale. To close this gap, we developed new ESM modules representing subgrid through stochastic parameterizations, trained and evaluated with high-resolution remote sensing data and site-level observations.

We will present novel results from in-situ experiments that quantify carbon fluxes and environmental response functions at patch-level within heterogeneous Arctic ecosystems, resulting in optimized strategies to integrate data streams for upscaling. Satellite remote sensing products investigate fine scale (few meters) patterns in Arctic landscapes that are undergoing modifications linked to climate change, including e.g. InSAR data to constrain ground ice content, and related subsidence patterns. Targets investigated include for example sinking surfaces, wetness gradients in heterogeneous landscapes, and drained lake basins. Assimilation of these new datasets supported the development of new ESM model components that successfully capture the statistics of small-scale features, including e.g. lateral connections between hydrologic landscape elements across scales, or thermokarst lake dynamics. Our results demonstrate that the ability to project the response of the high-latitude water, energy and carbon cycles to rising global temperatures may strongly depend on the ability to adequately represent the soil hydrology and disturbance effects in permafrost affected regions.

How to cite: Göckede, M., Bartsch, A., Brovkin, V., and Heimann, M. and the Q-Arctic Team: Q-Arctic: synergetic observations and modeling of pan-Arctic interactions between hydrology, disturbance and carbon cycle processes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13537, https://doi.org/10.5194/egusphere-egu26-13537, 2026.

EGU26-13606 | ECS | Posters on site | CR4.5

Using Ground Penetrating Radar to Estimate Talik Thickness Below the Kuparuk River, Arctic Alaska 

Samuel Lee, Rodrigo Correa Rangel, Thomas W. Glass, Aidan Armstrong, Benjamin M. Jones, and Ken D. Tape

Continued climate warming directly impacts regional hydrological systems through increased permafrost degradation and talik expansion. These disturbances alter surface and groundwater flow paths, increasing uncertainty in hydrological responses to future climate change. Previous research has observed groundwater flow in permafrost regions, either through suprapermafrost taliks or subpermafrost aquifers; however, a near-surface geophysical approach to quantify talik volume is required. We used Ground Penetrating Radar (GPR) data collected in March 2025 to estimate talik thickness below the Kuparuk River on the North Slope of Alaska. The Kuparuk River extends from the Brooks Range to the Beaufort Sea, making this region imperative for understanding the impacts of permafrost degradation on hydrological systems within the Arctic tundra.  GPR measurements were collected using a snowmobile pulling a 160 MHz antenna, reaching a depth of investigation up to ~30m. Preliminary GPR results suggest a talik layer below the river, which is hypothesized to facilitate groundwater flow during the winter. GPR talik thicknesses will be used to create a conceptual hydrogeological model of this complex river-talik system. This work provides a better understanding of the impacts of permafrost degradation on groundwater flow in an increasing climate warming.

How to cite: Lee, S., Rangel, R. C., Glass, T. W., Armstrong, A., Jones, B. M., and Tape, K. D.: Using Ground Penetrating Radar to Estimate Talik Thickness Below the Kuparuk River, Arctic Alaska, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13606, https://doi.org/10.5194/egusphere-egu26-13606, 2026.

EGU26-13826 | Orals | CR4.5

Pore size heterogeneity and groundwater flow as key factors contributing to subsea permafrost change in the Beaufort Sea 

Valentin Marguin, Gabriel Fabien-Ouellet, and Mathieu J. duchesne

Recent observations indicate that Arctic permafrost is warming and degrading rapidly. While the processes disrupting terrestrial permafrost are now relatively well documented, the dynamics of subsea permafrost on Arctic continental shelves remain poorly constrained. In particular, the combined influence of sedimentary heterogeneities and groundwater circulation remains largely underrepresented in current models. 
 
We present a multiphysical numerical modelling approach to better constrain the thermo-hydrological evolution of subsea permafrost in the Beaufort Sea. The model explicitly incorporates thermal conduction and advection, salinity transport, water-ice phase changes, and realistic sediment stratification (sand, silt, and clay) resulting from marine transgression and regression cycles during previous glacial-interglacial cycles. Our results show that lithology exerts a major control on the distribution of submarine permafrost. Clay-rich units, characterised by low permeability, have a drop in melting temperature depending on pore size (Gibbs–Thomson equation), leading to high spatial heterogeneity in the ice fraction, consistent with observations from recent seismic data. Conversely, sandy units, which are more permeable, can promote upward groundwater flows. Under conditions of negative seabed temperatures, these flows induce local desalination near the surface and the formation of new ice, consistent with recent field observations.
 
Our simulations include the last glacial–interglacial cycle (approximately 125 ka) and future warming scenarios, allowing us to evaluate both the glacial heritage and the transient response of the system to climate forcings. Comparing modelling results with drilling and seismic survey data, we provide a theoretical basis for interpreting field data. This study highlights the need to explicitly integrate sedimentary stratification and hydrogeological processes to reduce uncertainties about the future evolution of subsea permafrost and associated geological risks.

How to cite: Marguin, V., Fabien-Ouellet, G., and J. duchesne, M.: Pore size heterogeneity and groundwater flow as key factors contributing to subsea permafrost change in the Beaufort Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13826, https://doi.org/10.5194/egusphere-egu26-13826, 2026.

EGU26-13863 | ECS | Orals | CR4.5

Process-based modelling of active layer dynamics under changing Arctic precipitation: insights from Zackenberg, Greenland 

Laureen Ruge, Hannu Marttila, Efrén López-Blanco, and Julian Klaus

Arctic regions are undergoing rapid climatic change, including an increasing proportion of rain in annual precipitation. This change is expected to alter ground thermal regimes, permafrost stability, and soil hydrological processes. While previous studies have primarily focused on the effects of rising air temperatures on permafrost, the impact of changes in precipitation remains insufficiently quantified, given the variability and uncertainty of future precipitation projections.

This study evaluates the effects of altered precipitation patterns on active layer dynamics at Zackenberg, northeast Greenland. We combined long-term field observations with pedon-scale modelling using the CryoGrid community model, a coupled soil thermal-hydrological model that explicitly represents water and ice dynamics. We derived model parameters from site-specific measurements and calibration, and then validated their performance against independent observations. We obtained future precipitation scenarios from bias-corrected HIRHAM5 RCP4.5 and RCP8.5 projections.

The model reproduces the main hydrothermal dynamics of the active layer well. Simulation uncertainties remain due to simplified representations of percolation, snow insulation, and limited soil moisture data. Parameter evaluation reveals equifinality among evaporation depth, the evapotranspiration ratio, and saturated hydraulic conductivity. Uncorrected HIRHAM5 forcing exhibits a pronounced cold bias, resulting in underestimated active layer thickness (ALT) and emphasising the need for bias correction. High interannual variability in precipitation amount and rain–snow partitioning strongly influences both ALT development and freeze-back dynamics, largely independent of mean air temperature trends. Differences between RCP8.5 and a wetter, modified scenario suggest that wetter conditions can constrain active layer deepening under otherwise identical forcing, indicating that increased soil moisture may partially buffer warming effects. Our results show that uncertainties in precipitation projections have a major impact on active layer dynamics, providing process-based evidence that precipitation is a key driver in warming Arctic permafrost regions.

How to cite: Ruge, L., Marttila, H., López-Blanco, E., and Klaus, J.: Process-based modelling of active layer dynamics under changing Arctic precipitation: insights from Zackenberg, Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13863, https://doi.org/10.5194/egusphere-egu26-13863, 2026.

EGU26-13878 | ECS | Orals | CR4.5

Spatial variability of modern carbon burial in the Canadian Beaufort Sea  

Katharina Schwarzkopf, Lisa Bröder, Julie Lattaud, Michael Fritz, Volker Brüchert, Thomas Bosse-Demers, Bennet Juhls, Paul Overduin, Andre Pellerin, Daniel Rudbäck, Tommaso Tesi, Jorien Vonk, Dustin Whalen, and Matt O'Regan

Arctic continental shelves play a key role in the biogeochemical cycle by transporting and storing organic matter (OM) originating from permafrost, yet the spatial variability of sedimentation and OM accumulation remains poorly constrained. On the Canadian Beaufort Shelf, existing estimates of organic carbon (OC) storage are based on Holocene sedimentation rates derived from seismic data, while direct observations are rare and geographically limited (n=5). Here, we present new sedimentological and radiometric data from 17 sites spanning the Beaufort Shelf and continental slope. Measurements of total organic carbon, grain and dry density, as well as radionuclide profiles (210Pb, 226Ra, 137Cs), are used to estimate sediment accumulation, mass accumulation, and OC burial over the last ~150 years. Sedimentation rates derived from the Constant Flux-Constant Sedimentation (CF:CS) model are compared with those from a Bayesian 210Pb age modeling framework (rplum). CF:CS yields higher sedimentation rates (mean = 0.23 ± 0.15 cm yr-1) than rplum (mean = 0.17 ± 0.07 cm yr-1). Estimated OC burial rates range from 3.6 to 51.4 g m-2 yr-1, with the highest values found near the Mackenzie Delta and in the Kugmallit Trough. For shelf areas between 20-100 m water depth, our new data suggest average OC burial rates (24.4 g m-2 yr-1) that are three times higher than previously reported. Combined with shallow-shelf estimates, total carbon burial is revised to 1.44 Tg C yr-1, 75% higher than earlier estimates.

How to cite: Schwarzkopf, K., Bröder, L., Lattaud, J., Fritz, M., Brüchert, V., Bosse-Demers, T., Juhls, B., Overduin, P., Pellerin, A., Rudbäck, D., Tesi, T., Vonk, J., Whalen, D., and O'Regan, M.: Spatial variability of modern carbon burial in the Canadian Beaufort Sea , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13878, https://doi.org/10.5194/egusphere-egu26-13878, 2026.

The Smoking Hills (Ingniryuat) is a polar desert of Arctic Canada, which contains naturally occurring streams and ponds of hyper-acidic (pH < −2) metal-rich brines (total dissolved solids up to 394,000 mg/L). Acid waters are formed though oxidation of pyrite and metal-rich mudstones of the Late Cretaceous Smoking Hills Formation. Water in contact with the mudstones rapidly changes chemistry, becoming acidic, metal-rich, and opaque orange due to precipitation of Fe-sulfates. Acid generation occurs through mass wasting of Smoking Hills Formation mudstones due to permafrost thaw and ground ice melt in addition to coastal erosion and stream undercutting.  Fluvial incision through bedrock strata also leads to acid generation. These hyper-acidic metal-rich waters discharge to larger river systems and are transported to the Arctic Ocean, increasing some metal concetrations to exceed health guidelines for drinking water and skin contact. Climate warming will likely increase slumping rates and associated debris flows, impounding more surface ponds and stream courses, generating more acid waters, amplifying toxic metal flux to the environment, and drive river ‘rusting’.

How to cite: Grasby, S.: Release of toxic-metal acid-brines related to permafrost thaw driven slumping of Cretaceous mudstones – Smoking Hills (Ingniryuat), Arctic Canada, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14256, https://doi.org/10.5194/egusphere-egu26-14256, 2026.

EGU26-14381 | Orals | CR4.5

Coupled seepage-thermal effects and adaptation measures for an arctic bridge 

Greg Siemens and Astrid Schetselaar

Climate warming as well as anthropogenic effects are disturbing subsurface thermal and water regimes in northern regions. As an arctic nation, Canada continues to expand all-season transportation linkages to improve access to remote communities, natural resources, and emerging marine corridors. While these investments provide substantial societal, economic, and strategic benefits, the ground-infrastructure-climate interactions can prove complicated on the local and regional scale. The Inuvik–Tuktoyaktuk Highway (ITH), located within the continuous permafrost zone, is Canada’s first all-season road to reach the Arctic coast and represents an important transition toward climate-adaptive infrastructure design. The highway incorporates numerous drainage crossings where bridges are founded on deep foundations embedded in frozen ground.  Hans Creek Bridge, located at 57 km along ITH, is a three-span structure with abutments and piers founded on adfreeze piles in permafrost. Adfreeze pile foundations require cold temperatures (<-1oC) to support the overlying super-structure, making them highly sensitive to changes in ground temperature. The bridge as also constructed to be climate adaptation–ready, allowing for future installation of thermosyphons should mitigation become necessary. Ground temperature monitoring, correlated with near-surface geophysics, indicates that thermal conditions at the abutments are cooling as intended; however, temperatures of the pier foundations have increased over time, potentially due to localized groundwater seepage effects. This spatial variability highlights the importance of site-specific coupled thermal-seepage processes affecting the permafrost response. Preliminary coupled seepage-thermal modelling results indicate seepage velocities greater than approximately 1 cm / day could significantly reduce thermosyphon efficiency. Thermosyphon installation can be customized to increase effectiveness of passive ground cooling under complex thermal and hydrological conditions. The combined approach using ground temperature measurements and near surface geophysics as well as coupled seepage-thermal modeling highlights the coupled climate change–anthropogenic effects on critical arctic infrastructure and the owner’s plan to stave off these same effects.

How to cite: Siemens, G. and Schetselaar, A.: Coupled seepage-thermal effects and adaptation measures for an arctic bridge, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14381, https://doi.org/10.5194/egusphere-egu26-14381, 2026.

EGU26-15147 | Orals | CR4.5

Churning of the seafloor: On-going growth and collapse of ice cored submarine pingos 

Charles Paull, Giancarlo Toni, David Caress, Aaron Micallef, Jong Kuk Hong, Mathieu Duchesne, Eve Lundsten, Sebastian Rodríguez-Martínez, Roberto Gwiazda, Jennifer Paduan, Virgina Brake, Ji-Hoon Kim, and Seung-Goo Kang

A multipronged, 12-year study has revealed a complex, submarine morphology dotted with pingos which are continually changing due to ongoing freezing and thawing of brackish groundwater seeping up from buried ancient permafrost. Multibeam mapping surveys on both sides of the Mackenzie Trough in the Canadian Beaufort Sea were repeated in 2025, 8 and 12 years after the initial mapping surveys. Differencing 1-m-scale bathymetry grids collected using Autonomous Underwater Vehicles reveals the tops of pingos experience up to 1.5 m of upwards growth between surveys, documenting of upwards growth approaching 20 cm per year of submarine pingos for the first time. Up to 5 m of down drops were also observed on the crest of some submarine pingos. Areas that experience 1.5 m of growth are less than 10 m from areas that experienced 2.0 m of down drops. Remotely Operated Vehicle (ROV) based low altitude surveys using stereo cameras, multibeam, a laser scanner, and vision-based Simultaneous Localization and Mapping navigation mapped sections of this dynamic morphology at sub-cm resolution providing extraordinary detail on the on-going seafloor deformation associated with submarine permafrost. An ice layer exposed in the wall of an <8-year-old crater on the top of a pingo was sampled using a ROV-deployed drill. This ice sample and gravity cores show that segregated ice and ice bounded sediment exist at and just beneath the seafloor on these uplifted structures. Down-core freshening of pore waters from sediment cores taken on the tops of features also confirms that brackish water exists near the seafloor at these sites. ROV measurements show that the bottom water temperatures are <-1° C. At this temperature, fluctuating temperature and salinity of seeping brackish ground waters causes their freezing and thawing and results in the crest of ice cored pingos both growing and collapsing. This latest work broadens the known extent of active submarine permafrost deformation to include submarine pingos on the Arctic shelf. The on-going upwards growth and seafloor collapse at submarine groundwater seeps result in churning-up the seafloor and show that submarine permafrost formation represents an unanticipated geohazard threat to submarine infrastructure.

How to cite: Paull, C., Toni, G., Caress, D., Micallef, A., Hong, J. K., Duchesne, M., Lundsten, E., Rodríguez-Martínez, S., Gwiazda, R., Paduan, J., Brake, V., Kim, J.-H., and Kang, S.-G.: Churning of the seafloor: On-going growth and collapse of ice cored submarine pingos, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15147, https://doi.org/10.5194/egusphere-egu26-15147, 2026.

EGU26-15960 | ECS | Posters on site | CR4.5

Permafrost and shrubification: Friends or enemies? A look at the summer energy budget of shrub tundra 

Etienne Tremblay, Florent Domine, Antoine Thiboult, and Daniel Nadeau

Polar regions are warming about four times faster than the global average, favoring vegetation changes such as shrub expansion across Arctic tundra. Shrubification modifies the depth of the active layer, the summer-thawed layer whose magnitude affects the release of ancient organic carbon through microbial activity. In winter, snow insulates the ground from the atmosphere, but shrubs modify snowpack thermal properties and facilitate heat transfer through their branches. In summer, the relationship between shrub and ground thermal dynamics remains debated, with many interpretations focusing on shading effects by shrubs, but detailed surface energy budget studies are rare. This limits our ability to improve land surface models and quantify vegetation-permafrost feedbacks.

Here we compare summer surface energy partitioning of shrub and moss tundra in Qarlikturvik Valley on Bylot Island (73°N), Canadian High-Arctic.

From July 2024 to August 2025, we instrumented a low-shrub-dominated site and an adjacent moss-dominated site. We continuously monitored turbulent, radiative, and ground heat fluxes. We also characterized soil thermal properties and vegetation cover, and monitored snowpack thermal properties to help separate winter legacy effects from summer processes. Preliminary data show that ground temperatures are warmer annually under shrubs, with larger differences in winter. In summer, shrubs impact energy partitioning by modifying latent and sensible heat exchanges. Above the surface under the canopy, incoming shortwave radiation is attenuated. This reduced energy input is compensated by the thinner moss layer under shrubs which provides less thermal insulation and facilitates soil warming. By late summer, the active layer beneath shrubs is nearly twice as deep as at the moss site. This is mostly attributed to the winter legacy and to the lower moss insulation at our site.

This local study with a detailed dataset will contribute to improving vegetation-snow-permafrost parameterisations in land surface models and hopefully to more reliable Arctic permafrost projections.

How to cite: Tremblay, E., Domine, F., Thiboult, A., and Nadeau, D.: Permafrost and shrubification: Friends or enemies? A look at the summer energy budget of shrub tundra, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15960, https://doi.org/10.5194/egusphere-egu26-15960, 2026.

EGU26-16651 | ECS | Posters on site | CR4.5

A new process-based methanogenesis routine in the JSBACH land surface model – a pan-Arctic view of the CO2:CH4 ratio 

Marius Moser, Victor Brovkin, and Christian Beer

The Arctic is warming at an increased rate. This will lead to large-scale permafrost thaw, thereby potentially releasing significant amounts of greenhouse gases to the atmosphere through the decomposition of previously frozen organic material in the soils. To accurately gauge the impact of these emissions, it is crucial to know the emission ratio between the two most important greenhouse gases CO2 and CH4. While CO2 is projected to be the dominant gas, it is important to consider the amplified climatic forcing of CH4, which is a stronger greenhouse gas than CO2. Laboratory incubations and in situ studies have shown that the CO2:CH4 ratio is highly variable. Despite this, most land surface models use a pre-set ratio factor to simulate methanogenesis, thus making it impossible to capture the dynamics of the CO2:CH4 ratio from the start, and, in consequence, making prediction of the Arctic carbon budget more uncertain. Methanogenesis is a complicated framework of different microbial processes, most importantly the two main production pathways – acetoclastic and hydrogenotrophic methanogenesis – and fermentation, which produces the substrate for the two former processes. The inclusion of these processes into models has been studied on the small, i.e. lab to site-level, scale but this has rarely been explored on a pan-Arctic scale. Here, we augmented the JSBACH land surface model’s methane routine, which normally uses a predefined CH4 production ratio factor, by including the three aforementioned microbial processes to study the CO2:CH4 ratio on a pan-Arctic scale. We present the new model routine, show how it performs against the base model, and how the results compare to other estimates from the literature. We discuss the uncertainty of the new results and highlight the difficulties in upscaling many of the factors that influence the CO2:CH4 production ratio.

How to cite: Moser, M., Brovkin, V., and Beer, C.: A new process-based methanogenesis routine in the JSBACH land surface model – a pan-Arctic view of the CO2:CH4 ratio, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16651, https://doi.org/10.5194/egusphere-egu26-16651, 2026.

EGU26-16782 | ECS | Posters on site | CR4.5

Northern hemisphere permafrost loss documented through ESA CCI+ Permafrost climate data records 

Chiara Gruber, Annett Bartsch, Sebastian Westermann, and Tazio Strozzi

The objective of the European Space Agency Climate Change Initiative (ESA CCI+) Permafrost project is to develop and deliver permafrost data as Essential Climate Variable (ECV) products primarily derived from satellite measurements (https://climate.esa.int/en/projects/permafrost/). The required associated parameters by the Global Climate Observation System (GCOS) for the ECV Permafrost are 'permafrost temperature' and 'active layer thickness'. Further on, permafrost extent (as a derivative of ground temperature) needs to be quantified.

Algorithms were identified which can provide these parameters of interest by ingesting a set of global satellite data products (land surface temperature and land cover), re-analysis data (snow-water equivalent) and subsurface stratigraphy in a permafrost model scheme that computes the ground thermal regime.

The resulting datasets are annual products of mean annual ground temperature (MAGT) at different depths, active layer thickness (maximum thaw depth) and permafrost fraction (based on MAGT at 2m depth) from 1997 to 2023.

The estimated reduction of permafrost extent in the timeframe from 1997 to 2023 was 8%. The mean annual ground temperature at 2m depth has increased from approximately -2°C to -1°C (within maximum permafrost extent of the observation period). The thickness of the active layer has increased by 30 cm on average. Distinct regional differences can be observed which will be presented.

How to cite: Gruber, C., Bartsch, A., Westermann, S., and Strozzi, T.: Northern hemisphere permafrost loss documented through ESA CCI+ Permafrost climate data records, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16782, https://doi.org/10.5194/egusphere-egu26-16782, 2026.

EGU26-16840 | Posters on site | CR4.5

Satellite based monitoring of Arctic settlements on thawing ground 

Barbara Widhalm, Annett Bartsch, Rustam Khairullin, Clemens von Baeckmann, Rodrigue Tanguy, Tom De Ville, and Thomas Ingeman-Nielsen

Infrastructure in the Arctic is expanding rapidly due to ongoing industrial development, yet it faces increasing challenges as climate warming accelerates permafrost degradation and leads to or increases ground instability. Satellite records support the identification of infrastructure developments. Remote sensing based ground surface deformation monitoring is another key component for managing permafrost-related infrastructure risks and supporting community planning.

To systematically map human-impacted Arctic coastal regions, the Sentinel-1/2 derived Arctic Coastal Human Impact (SACHI) dataset was developed. In this study, we updated this dataset for selected Arctic settlements in western Greenland using newly acquired imagery that captures recently constructed man-made features. Additionally, we investigated the potential of fully polarimetric PALSAR-3 L-band SAR data to complement the established Sentinel-1 (C-band)/ Sentinel-2 workflow, aiming to improve the detection and characterization of infrastructure. The scheme is based on fusion of two machine learning techniques, Gradient boosting machines (GBM) and a deep learning approach using convolutional neural networks. Specifically, the added value for building detection as part of the GBM analyses can been shown. Eventually we combined the settlement information with long-term vertical ground deformation for selected settlements.

How to cite: Widhalm, B., Bartsch, A., Khairullin, R., von Baeckmann, C., Tanguy, R., De Ville, T., and Ingeman-Nielsen, T.: Satellite based monitoring of Arctic settlements on thawing ground, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16840, https://doi.org/10.5194/egusphere-egu26-16840, 2026.

EGU26-16924 | Posters on site | CR4.5

Differentiation of Drained Lake Basin Types considering river floodplains 

Clemens von Baeckmann, Annett Bartsch, Helena Bergstedt, Barbara Widhalm, Rustam Khairullin, Tobias Stacke, and Philipp De Vrese

The Arctic permafrost is warming widely, and the circumpolar region is heating up four times faster than the global average. Common features of permafrost landscapes are drained lake basins (DLBs) which play an important role for the geomorphological, hydrological and the ecological development of those landscapes. In addition, rivers transport significant amounts of freshwater, dissolved organic carbon, and other materials into the Arctic Ocean. The impact of close-by streams for DLB drainage and refilling events needs to be quantified.

Here, we focus on DLBs and their connections to river floodplains on the Yamal Peninsula in northern Siberia, a region underlain by both discontinuous and continuous permafrost and covered with tundra vegetation, thaw lakes, and wetlands. For this study, we investigated manually selected DLBs using DEM derivatives. The lakes represent a North-South climatic gradient and different drained lake basin development stages. DEM derivatives are also used to represent related small-scale landscape features in climate models. The utility of metrics based on the Copernicus DEM, which were recently implemented in the ICON-Land model, was assessed. Potential floodplain linkage could be identified in many cases, leading also to diverting patterns of landcover evolution after drainage.

The results provide a foundation for further analysis of lakes and their connections to streams, which play a role in the wetting and drying processes and subsequent impacts on the carbon cycle across the Arctic.

How to cite: von Baeckmann, C., Bartsch, A., Bergstedt, H., Widhalm, B., Khairullin, R., Stacke, T., and De Vrese, P.: Differentiation of Drained Lake Basin Types considering river floodplains, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16924, https://doi.org/10.5194/egusphere-egu26-16924, 2026.

EGU26-17317 | Orals | CR4.5

Wildfires accelerate permafrost area loss via reducing soil organic matter 

Dan Zhu, Yining Zhang, Zhen Wang, Yiqin Chen, Philippe Ciais, and Tao Wang

The stability of permafrost is regulated by the thermal insulating properties of soil organic carbon (SOC). However, intensifying wildfires across the Arctic and boreal regions are removing the protective soil organic layer, which may trigger positive feedback that accelerates thaw, yet the pan-Arctic scale of this threat remains unknown. Here we present a data-driven framework, aiming to address two questions: i) what is the net SOC loss due to fire across the northern permafrost zones, accounting for immediate SOC combustion and post-fire recovery, and ii) to what extent does this fire-induced SOC reduction accelerate permafrost degradation. To achieve this, we developed a bookkeeping model parameterized by SOC data from over 1,000 paired burned and unburned sites across diverse ecosystems to simulate fire-induced SOC dynamics, and a permafrost probability model based on air temperature and SOC content, advancing earlier temperature-only approaches. Driven by CMIP6 climate and burned area projections, we find that under SSP1-2.6, fire-induced SOC loss, considering both combustion and post-fire recovery, reaches 15.0±3.6 Pg C by 2100. This SOC reduction diminishes the soil’s insulative capacity, leading to an additional permafrost loss of 2.7±0.7 million hectares. This impact is most pronounced under low-emission scenarios, where permafrost exists in a climatically marginal state; here, every 1 km² of increased burned area causes 0.19 km² of additional permafrost loss. Under SSP5-8.5, fire-driven permafrost loss is less pronounced as rapid atmospheric warming is the predominant driver. Our findings reveal that wildfire is an efficient agent of permafrost thaw, highlighting the urgent need to incorporate dynamic fire-SOC-thermal interactions into ESMs to avoid underestimation of future permafrost degradation.

How to cite: Zhu, D., Zhang, Y., Wang, Z., Chen, Y., Ciais, P., and Wang, T.: Wildfires accelerate permafrost area loss via reducing soil organic matter, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17317, https://doi.org/10.5194/egusphere-egu26-17317, 2026.

EGU26-18289 | ECS | Posters on site | CR4.5

Assessing the tundra-boreal transition zone with Sentinel-1/2–derived landcover data 

Rustam Khairullin, Annett Bartsch, and Birgit Heim

Geographical and ecological research of Arctic tundra requires a clear definition of the biome boundaries. A commonly used dataset for the Arctic is the tundra biome boundary mapped by the Circumpolar Arctic Vegetation Mapping Project (CAVM, 2003). Given recent advances in satellite-image resolution and data availability, in the age of the rapidly changing Arctic climate this previously established delineation needs to be re-evaluated and, where necessary, updated. An updated boundary can support applications such as Arctic climate modelling and assessments of potential disturbances in permafrost rich regions.

A recently developed landcover dataset was investigated for this study. The Circumpolar Landcover Unit (CALU) Database provides highly detailed landcover information with a spatial resolution of 10 meters and consists of 23 thematic units, including 12 units representing tundra but also 3 forest classes. The used retrieval scheme of landcover units employed provides an unprecedented level of detail. The landcover units have been derived by fusion of satellite data using Sentinel-1 (synthetic aperture radar) and Sentinel-2 (multispectral). These units reflect gradients in moisture and vegetation structure. The available spatial detail of CALU has been already shown to provide the means to assess the complexity of lowland permafrost regions.

The original CALU database of version 1.0 covered the Arctic within the CAVM extent only. The latest version 2.0 partially extends further south, providing additional detail within the transition zone for many areas.

The aim of this study was to assess the southern boundary of the CAVM and to identify regions where further developments of the CALU dataset may aid to establish a new boundary. Spatial statistics were collected within selected buffer areas of the CAVM boundary. In addition, longitudinal zones were generated to test whether forest-related CALU classes systematically peak south of the currently mapped boundary.

Based on these statistics, in regions such as Alaska and the European part of Russia, the CAVM boundary generally corresponds well with CALU, with forest-related classes mostly dominating within the buffer area. In parts of Siberia and Canada, however, shrub-tundra classes are more prevalent, while forest-related classes occur farther south. This mismatch may reflect regional differences in vegetation structure and terrain-driven zonation, suggesting that a single latitudinal boundary product may not capture local transitions equally well everywhere.

Preliminary results indicate that in several regions the CALU database should be extended further south, because current coverage does not fully include forest-related classes. This limitation affects the use of CALU for the tundra-boreal biome boundary evaluation and for applications that require a consistent representation of tundra–taiga transitions.

CALU: Bartsch, A., Khairullin, R., Efimova, A., Widhalm, B., Muri, X., von Baeckmann, C., Bergstedt, H., Ermokhina, K., Hugelius, G., Heim, B., Leibman, M., & Gruber, C. (2024). Circumarctic Landcover Units (2.0) [Data set]. Zenodo. https://doi.org/10.5281/zenodo.14235736

How to cite: Khairullin, R., Bartsch, A., and Heim, B.: Assessing the tundra-boreal transition zone with Sentinel-1/2–derived landcover data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18289, https://doi.org/10.5194/egusphere-egu26-18289, 2026.

EGU26-19294 | ECS | Orals | CR4.5

Permafrost thaw increases CH4 fluxes in disturbed Yedoma tundra landscapes in Western Alaska  

Mackenzie Baysinger, Wasi Hashmi, Cornelia Inauen, Guido Grosse, Caitlynn Hanna, Tillmann Lübker, Aleksandra Veremeeva, Tina Sanders, Maija Marushchak, and Claire Treat

Permafrost thaw features –such as thermokarst lakes, retrogressive thaw slumps, and thermo-erosional gullies– are becoming increasingly widespread across the Arctic as a direct result of warming global temperatures. Permafrost underlies 15% of the land surface area in the Northern Hemisphere, and globally is estimated to store substantially more carbon (1,300 Pg of C) than all the world's forests. Despite the massive amount of permafrost soil carbon, little is known about the processes that spur microbial respiration as the soils transition to a post-thaw state, resulting in increased contributions of greenhouse gas emissions. Understanding these processes is particularly important in regions underlain by late Pleistocene, ice-rich Yedoma deposits that contain large amounts of buried, poorly decomposed organic matter. To investigate the potential greenhouse gas (GHG) contribution of these thaw features in Yedoma landscapes, we sampled carbon dioxide and methane gas fluxes across eight thaw transects on the Baldwin Peninsula (Western Alaska) in the summers of 2023 and 2024. We used manual chamber measurements to measure the in-situ GHG fluxes and recorded site parameters to categorize the extent of thaw disturbance (including topography, active layer depth, soil moisture, vegetation, and more). 

 

From these measurements, we found that permafrost thaw increased CH4 fluxes exponentially relative to adjacent undisturbed tundra, with mean fluxes ranging from 0.6 to 7.0 mg CH4-C m-2 d-1 and 25.6, 67.4, 71.9 mg CH4-C m-2 d-1 in recently drained thermokarst lake basins, thaw ponds, and thermo-erosional gullies, respectively. Almost all sites were net sources of methane to the atmosphere, with the exception of two upland measurements in minimal thaw disturbance landscapes (CH4 fluxes were < -0.3 mg CH4 m-2 d-1 representing net CH4 oxidation). Across all landscapes included in the sampling, retrogressive thaw slumps, representing freshly exposed Yedoma deposits, had the highest mean CH4 flux among the other disturbed permafrost landforms (159 mg CH4-C m-2 d-1). Though undisturbed upland sites are generally thought to be net sinks of carbon, our measurements show that methane emissions were ubiquitous – even in well aerated sites, suggesting complex or inhomogeneous subsurface conditions. In these undisturbed sites, ecosystem respiration fluxes from sites that had vegetation were not significantly different than those with bare soil, suggesting that it was not the upland plant life driving net GHG patterns. Rather, we propose that the underlying carbon-rich Holocene soils and late Pleistocene Yedoma deposits provide a consistent trickle of methane and CO2 to the surface. This study provides field data on CH₄ and CO₂ fluxes across multiple thaw landforms in a Western Alaska Yedoma landscape, highlighting the potential role of deep carbon mobilization across a gradient of disturbance.

How to cite: Baysinger, M., Hashmi, W., Inauen, C., Grosse, G., Hanna, C., Lübker, T., Veremeeva, A., Sanders, T., Marushchak, M., and Treat, C.: Permafrost thaw increases CH4 fluxes in disturbed Yedoma tundra landscapes in Western Alaska , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19294, https://doi.org/10.5194/egusphere-egu26-19294, 2026.

EGU26-19823 | Posters on site | CR4.5

Understanding Soil Freeze-Thaw Dynamics and Slope Instability in Arctic Regions Under Climate Change 

Mirela Vasile, Kimmo Rautiainen, Manu Holmberg, Marina Vârghileanu, Nicolas Alexandru, and Ionuț Șandric

Climate-driven transitions in Arctic soil states, from frozen to intermediate and thawed conditions, pose significant threats to slope stability in permafrost regions. As permafrost degrades, slope structural integrity weakens, elevating landslide risk and other geohazards. This study analyzes long-term trends in soil freeze-thaw dynamics across the Arctic to identify areas vulnerable to future slope instability and inform infrastructure planning, resource management, and hazard mitigation strategies.

We utilized SMOS brightness temperature data from the CATDS dataset and SMOS L3 Freeze-Thaw State products from ESA, analyzing normalized polarization ratio (NPR) and freeze-intermediate-thaw (FT) classifications from both ascending and descending orbits. Trend detection employed two complementary approaches: the Mann-Kendall non-parametric test for monotonic trends and Long Short-Term Memory (LSTM) neural networks for capturing complex temporal patterns. Analyses were conducted at monthly and seasonal scales across individual pixels and spatial clusters (3×3, 5×5, and 7×7 pixels).

Results reveal pronounced changes clustered in northern Canada, Alaska, Siberia, and Arctic Ocean coastal zones. These regions display heterogeneous patterns reflecting localized frost condition shifts. Northern Canada and Alaska show trends consistent with permafrost degradation driven by rising temperatures and seasonal frost variations. Siberian trends suggest accelerating permafrost thaw with implications for carbon release, ecosystem function, and infrastructure integrity. Coastal Arctic zones exhibit changes linked to sea ice retreat, coastal erosion, and permafrost-climate interactions.

This research demonstrates the value of combining statistical and artificial intelligence methods to monitor environmental change in permafrost landscapes, providing critical insights for understanding slope instability drivers in a warming Arctic.

Acknowledgement: This work was supported by the European Union's Horizon 2020 programme (Grant No. 101086386, EO-PERSIST).

How to cite: Vasile, M., Rautiainen, K., Holmberg, M., Vârghileanu, M., Alexandru, N., and Șandric, I.: Understanding Soil Freeze-Thaw Dynamics and Slope Instability in Arctic Regions Under Climate Change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19823, https://doi.org/10.5194/egusphere-egu26-19823, 2026.

EGU26-20920 | Posters on site | CR4.5

Slowing down permafrost degradation: Quantifying the thermal buffer effect of the transient layer from novel large-scale laboratory experiments 

Calvin Beck, Emmanuel Léger, François Costard, Albane Saintenoy, Antoine Séjourné, François Duhayon, and Mikael Lasseigne

Permafrost is receding and warming globally in polar and high-altitude regions due to ongoing climate change. To better represent the role of ground ice on the long-term stability of permafrost soils, previous studies have introduced a transition zone between the seasonally freezing and thawing active layer and the permafrost layer. The transient layer, an ice-rich layer within the transition zone, is proposed to have the potential to temporarily slow down the climate change-related permafrost thaw. The ice-water phase transition absorbs heat and temporarily buffers the downward heat propagation. However, so far this layer has not received much scientific attention and its formation and degradation processes and their associated timescales remain largely unconstrained.

To determine the physical degradation processes of the transient layer as well as the involved time frame, we present a novel experimental approach to replicate the transient layer degradation under controlled laboratory conditions. The experimental setup at the GEOPS cold chamber facility consists of an acrylic glass container (approximately 80 × 40 × 40 cm, H × W × L). It is filled with fully saturated sand (d50 = 0.2 mm) or polycarbonate analog (d50 = 0.6 mm) material. The lateral boundaries of the container are insulated to minimize horizontal heat exchange, while the base of the container is kept at a constant temperature with a cryostat to represent the underlying permafrost. By cyclically varying the air temperature in the cold chamber between -30 °C and +30 °C we forced repetitive freeze-thaw cycles on the surface of the volume to simulate a permafrost system. To simulate the transient layer we have added different artificial cryostructures (ice lenses, ice veins, and dispersed ice) at the active-layer and permafrost layer interface. We varied the cryostructure type between experimental runs but kept the total ice-mass to keep the latent heat capacity constant. Then, to degrade the transient layer we increased the temperature forcing by shifting the temperature cycle upward by 3 °C. We monitored the transient layer degradation with an array of temperature sensors, a ground-penetrating radar, and photographic observations through the transparent side walls of the experimental container.

In this initial work, we show how different ice contents, spatial distributions, and cryostructure types within the transient layer protect the underlying permafrost beyond the latent-heat buffering of the ice-water phase transition alone. We highlight the importance of expanding the future use of these analog experiments to better understand and isolate the physical transient layer formation and degradation processes. This is essential in determining the transient layer evolution and its long-term implications for permafrost retreat and destabilization.

How to cite: Beck, C., Léger, E., Costard, F., Saintenoy, A., Séjourné, A., Duhayon, F., and Lasseigne, M.: Slowing down permafrost degradation: Quantifying the thermal buffer effect of the transient layer from novel large-scale laboratory experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20920, https://doi.org/10.5194/egusphere-egu26-20920, 2026.

EGU26-21908 | ECS | Posters on site | CR4.5

Setting up and parametrising a thermo-erosional gully model to study the impact of morphology and snowdrift on development trajectories 

Cornelia Inauen, Moritz Langer, Suzann Ohl, Alexandra Veremeeva, Anne Morgenstern, Tabea Rettelbach, Sambit Ghosh, Thomas Opel, Carlos Palacin-Lizarbe, Fabian Seemann, Sophia Barth, Mackenzie Baysinger, Caitlynn Hanna, Tillmann Luebker, Alexandra Runge, Ingmar Nitze, Irena Hajnsek, and Guido Grosse

Thermo-erosional gullies are widespread landscape components in ice-rich Arctic permafrost regions. With accelerated climate warming and permafrost thaw, these gully networks are expected to expand. This not only accelerates in-situ ground-ice loss but also rearranges drainage pathways, which can have far-reaching consequences, modifying local hydrology as well as sediment, nutrient, carbon, and contaminant fluxes and impacting ecosystems at catchment scale.

The evolution of thermo-erosional gully systems following initiation is dynamic and likely influenced by incision-dependent snowdrift and moisture redistribution that affect the thermal conditions. To investigate the role of these factors and their consequences for the permafrost state within the gully and the surrounding uplands, we set up a simplified thermo-erosional gully model using the permafrost model CryoGridLite, including conductive heat transfer, soil water phase change, a dynamic snow scheme and simplified water redistribution. The model was parameterised and validated to represent two contrasting gully sites in western Alaska, using field data. The first site on the Baldwin Peninsula (BAP-B) represents a deeply incised coastal gully, while the second site on the Seward Peninsula (CSP-F) represents a shallow gully connected to a drained thermokarst pond basin. The data included topographical measurements with drone-based measurements of terrain elevation and DGPS measurements of elevation transects for the morphological setup and snow depth measurements along cross-gully transects to constrain asymmetric snowdrift. For additional parametrisation and validation, we used various in-situ measurements, including temperature depth-profiles and thaw depth from several field campaigns (2022 to 2025), as well as continuously measured temperatures along gully cross-transects (upland, slope gully base) at different depths (surface, 0.2 to 0.3m, and 1 m). Based on the validated model setups for both sites, we modified morphology and snowdrift constraints to compare temperature dynamics and permafrost state along the gully cross section under different setup scenarios.

Our modelling scenarios highlighted the importance of snowdrift for talik formation within the gully. Furthermore, the model simulations suggest increased seasonal thaw depths on the slopes, which may result in enhanced mass wasting and erosion-driven gully widening and, together with directional snowdrift, lead to asymmetric gully development. Finally, we conclude that such storyline simulations can provide valuable insights into potential future development trajectories under climate change and address open questions such as the role of thermo-erosional gullies in permafrost landscapes. This includes whether gullies stabilise upland permafrost through improved drainage or whether related topographical changes enhance snow accumulation, thereby accelerating permafrost degradation.

How to cite: Inauen, C., Langer, M., Ohl, S., Veremeeva, A., Morgenstern, A., Rettelbach, T., Ghosh, S., Opel, T., Palacin-Lizarbe, C., Seemann, F., Barth, S., Baysinger, M., Hanna, C., Luebker, T., Runge, A., Nitze, I., Hajnsek, I., and Grosse, G.: Setting up and parametrising a thermo-erosional gully model to study the impact of morphology and snowdrift on development trajectories, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21908, https://doi.org/10.5194/egusphere-egu26-21908, 2026.

EGU26-2311 | Orals | GM9.1

Sub-monthly to inter-annual Arctic gravel beach change and controlling factors 

Zuzanna Swirad, Agnieszka Herman, and Mateusz Moskalik

Sixteen uncrewed aerial vehicle (UAV) surveys were conducted along a 2.5 km stretch of coastline of Isbjørnhamna, Hornsund, Svalbard during summer months between 2018 and 2025 to quantify topographic change within a gravel beach neighboring the Polish Polar Station (PPS) from days to years. Spectral wave model of Herman et al. (2025) was used to extract hourly nearshore significant wave height, peak period, energy period and wave energy flux. The model was validated against observational data of Swirad et al. (2023). Storms were extracted as events when significant wave height exceeded 95th percentile. Near-daily high-resolution ice/open water maps of Swirad et al. (2024) were used to create timeseries of ice coverage in the main basin of Hornsund and in Isbjørnhamna. Hourly wave runup was calculated for 10 m alongshore blocks using wave parameters, beach topography and an empirical runup formula developed by Poate et al. (2016) for gravel beaches. Wave runup combined with water level was used to extract timing of wave overtopping and coastal flooding.

We observed a great inter-annual variability in wave and ice conditions with the icy 2019/20 and 2021/22, the stormy 2018/19, 2020/21 and 2022/23, and the moderate 2023/24 and 2024/25. There was a great variability in volumetric coastal change with near-zero change after 7 years. Erosion focused in some hotspots, notably the vicinity of the PPS infrastructure, while the eastern part of the analysed beach experienced net deposition. At the sub-monthly to monthly scales high rates of coastal change were related to beach erosion by moving growlers, development of beach cusps, melting of ice buried under beach sediments and hydrological processes. 

References:

Herman A., Swirad Z.M. & Moskalik M. 2025. Increased exposure of the shores of Hornsund (Svalbard) to wave action due to a rapid shift in sea ice conditions. Elementa: Science of the Anthropocene 13(1): 00067. https://doi.org/10.1525/elementa.2024.00067

Poate T.G., McCall R.T. & Masselink G. 2016. A new parameterisation for runup on gravel beaches. Coastal Engineering 117: 176–190. https://doi.org/10.1016/j.coastaleng.2016.08.003

Swirad Z.M., Moskalik M. & Herman, A. 2023. Wind wave and water level dataset for Hornsund, Svalbard (2013–2021). Earth System Science Data: 15, 2623-2633. https://doi.org/10.5194/essd-15-2623-2023

Swirad Z.M., Johansson A.M. & Malnes E. 2024. Extent, duration and timing of the sea ice cover in Hornsund, Svalbard, from 2014–2023. The Cryosphere 18: 895-910. https://doi.org/10.5194/tc-18-895-2024

How to cite: Swirad, Z., Herman, A., and Moskalik, M.: Sub-monthly to inter-annual Arctic gravel beach change and controlling factors, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2311, https://doi.org/10.5194/egusphere-egu26-2311, 2026.

Permafrost is one of the main components of the cryosphere. Due to global warming, water frozen reservoir shrinking and a large number of natural hazards (debris flows, water quality deterioration, etc.) related to permafrost degradation are increasing. The permafrost mapping of the Gaizi River Basin located in the East Pamir where the significant Karakoram Highway traverses was important for understanding the situation of its water resource and related hazards. Three machine learning models (Artificial Neural Network, ANN; Random Forest, RF; Extreme Gradient Boosting, XGBoost), were trained to generate permafrost probability distribution based on rock glaciers from Chinese Gaofen-1. Rock glaciers are commonly used as direct indicators of mountain permafrost distribution, particularly in alpine regions with limited in-situ data. Sixteen independent factors were used for permafrost distribution mapping that includes elevation, aspect, slope, solar radiation, topographic roughness index, topographic wetness index, profile curvature, distance from rivers, distance to glaciers, distance to water bodies, geology, fault density, LULC, NDVI, precipitation, temperature difference. The performances of the models have been evaluated by the area under the receiver operating characteristic curve (AUROC) and by known rock glaciers. Random Forest outperformed other two models, with Receiver Operating Characteristic curve values of 0.97. The permafrost map covers almost all the rock glaciers (98%), which also shows the permafrost map is reasonable. The permafrost distribution covers 1853 km2, about 16.81% of the total river basin, mainly between 3233 and 5026 m elevation. The results could be used as baseline information for studying the impact of permafrost degradation and its related hazards because of climate warming, which threaten the Karakoram Highway.

How to cite: Liu, Y.: Permafrost distribution mapping using rock glaciers data and machine learning models in the Gaizi River Basin, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3822, https://doi.org/10.5194/egusphere-egu26-3822, 2026.

EGU26-4125 | ECS | Orals | GM9.1

Erodibility of frozen riverbed sediments 

Sjoukje de Lange, Jonas Eschenfelder, and Shawn Chartrand

Cryosphere degradation due to climate change results in increased sediment availability, mobilization, and transport (Knight & Harrison, 2012; Lane et al., 2017; Micheletti & Lane, 2016; Beel et al., 2020; Li et al., 2021a; Zhang et al., 2021; Syvitski et al., 2022; Zhang, 2022). The change in magnitude and timing of water delivery and sediment transport alters river patterns (Lafrenière & Lamoureux, 2019; Fortier et al., 2007), such as via increasing channelization (Liljedahl et al., 2016; Li et al., 2021a; Chartrand et al., 2023). Despite the obvious signs of landscape transformation by rivers, the effects of climate change on High Arctic fluvial incision and sediment transport remain poorly quantified due to limited understanding of how thawing substrate, water availability, and erodibility interact.

Although frozen landscapes are expected to erode slower than their temperate counterparts, Eschenfelder et al. (in review) found that frozen riverbeds may erode faster. In their laboratory flume experiments, they observe injections of surface water into a frozen bed of uniform-sized spherical glass beads (D50 of ~1.9 mm), delivering heat and momentum fluxes to the thaw front. This increased subsurface melting and drove development of pressure gradients which enhanced surface erosion. They argue that later in the thaw season, when the upper layer of the bed has thawed in a more homogeneous fashion, water injections into the bed are physically accommodated and hence do not contribute to elevated surface erosion.

The glass bead substrate of Eschenfelder’s experiments has a high porosity (p = 0.4) and permeability, supporting significant hyporheic flow. However, natural sediments vary in size and composition, altering porosity and permeability. Furthermore, sediment size variability affects thawing rate (Gatto, 1995; Costard et al., 2003, 2014) and erosion rate (Einstein, 1950, Mitchener & Torfs, 1996; McCarron et al., 2019; van Rijn, 2020; de Lange et al., 2024).

In the proposed follow-up experiments, we plan to use various mixtures of glass beads (D50 = 0.88, 1.9 and 4.1 mm), and natural sediments, to alter porosity and permeability. The natural sediment distribution will be scaled to reflect substrate compositions observed during past field campaigns to the Canadian Arctic. We hypothesise that, if these water injections into the bed are still present in lower porosity sediments, fine grained beds will erode slower than courser grained beds, despite a lower threshold of motion. Furthermore, experiments with multiple freeze-thaw cycles will be performed, allowing assessment of a potential positive feedback loop where past-seasons’ thaw front undulations and surface topography can impact current season’s flow patterns – imparting “memory” onto the landscape.

With these experiments we will assess erosional mechanisms in a variety of grain sizes, allowing us to further explore the mechanisms of erosion in frozen riverbeds, ultimately aiding the understanding of spatial variability in channel incision in the field.

How to cite: de Lange, S., Eschenfelder, J., and Chartrand, S.: Erodibility of frozen riverbed sediments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4125, https://doi.org/10.5194/egusphere-egu26-4125, 2026.

EGU26-5849 | ECS | Posters on site | GM9.1

A Physical Model of Permafrost Sorted Stripe Formation in the Canadian High Arctic 

Grace E. Johnson, Shawn M. Chartrand, and A. Mark Jellinek

Hillslopes in the Canadian High Arctic can express curious quasi-linear sorted stripe patterns, physically resembling rills but with no obvious evidence of active particle transport via sustained surface water flows following rainfall or snowmelt. This motivates several questions which at present are little explored. First, how do the physical characteristics of the pattern vary down the hillslope in response to changing hillslope geomorphology (e.g. slope, elevation, etc.)? Second, what mechanism(s) causes sorted stripe patterns to initiate and develop, and what are the roles of freeze-thaw, granular, and fluid-flow-driven processes? Several attempts have been made to model the formation of sorted stripe patterns using rules-based approaches, or analytical models derived from these rules; however, a comprehensive physical model of sorted stripe formation has yet to be developed, and we currently lack even a characterization of how the pattern is distributed across a hillslope.

Here, we present a characterization of the sorted stripe patterning found on a hillslope on Tallurutit (Devon Island), Nunavut and examine topographic controls of hillslope track characteristics. By analyzing topographic lidar data, we find that there is not one preferred cross- or downslope spacing of the stripes; rather, the size and shape of stripes varies down the hillslope. This alludes to the idea that there are several processes at work to form hillslope sorted stripe patterns. We present a physical model of stripe formation involving initial fracturing of the hill due to thermal stresses, heaving from ice lens growth, and mobilization of stones due to the creation of critically-steep topographic gradients and ice needle formation. We motivate this model using the characterization of the sorted stripe pattern distribution, field observations, and an analysis of thermal and tensional stresses.

How to cite: Johnson, G. E., Chartrand, S. M., and Jellinek, A. M.: A Physical Model of Permafrost Sorted Stripe Formation in the Canadian High Arctic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5849, https://doi.org/10.5194/egusphere-egu26-5849, 2026.

EGU26-5863 | ECS | Posters on site | GM9.1

Exposed! Paraglacial Drama Unfolding at Hørbyebreen, Central Svalbard 

Divya Nautiyal and Jan Kavan

Central Svalbard experiences one of the fastest warming trends in the Arctic and local glaciers are consequently retreating fast leaving behind vast forefields. As the glacier is not in the vicinity, it is not the glaciers that transforms the forefield but the paraglacial processes that work to continuously reshape them.

Here, we studied paraglacial processes in the Hørbye forefield by quantifying changes in the glacier extent, forefield geomorphology and formation/ drainage of the kettle lakes of the Hørbye glacier since the last mapping conducted in 2009. Aerial photography, UAV-based orthophotos and DEMs and field observations were employed to interpret forefield development.

Results of the study show an increased forefield size of Hørbyebreen since the last mapping in 2009.  The glacier has treated by 101237.4 m2. The area of the kettle lakes underwent a net decrease, with 68% of the total lakes either being drained, shrinking, or disappearing entirely due to sediment infilling from the fluvial plain. We also observed fluvial erosion of glacial landforms such as eskers.

Understanding these changes highlight the central role of paraglacial processes in post-retreat development. As the glacier moves to steeper topography, the retreat is expected to slow down, although the glacier will continue to provide enough water for intensive fluvial processes in the forefield. Widening of the sandur will lead to lateral erosion of the lakes in its vicinity. For the rest of the forefield, hydrological connectivity can reshape the existing network of lakes.

The changes observed between 2009-2024 show the retreat of the glacier front and changes in the geomorphological structures of the forefield. We observed a decline in the number of lakes and increase in the areal extent of the fluvial landforms.

How to cite: Nautiyal, D. and Kavan, J.: Exposed! Paraglacial Drama Unfolding at Hørbyebreen, Central Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5863, https://doi.org/10.5194/egusphere-egu26-5863, 2026.

EGU26-5879 | ECS | Posters on site | GM9.1

Holocene climate variability as reconstructed from 10Be dated glacial and periglacial phases in the Subtropical Andes 

Javiera Carraha, Juan Luis García, Hans Fernández-Navarro, and Dominik Amschwand

Despite major advances in paleoclimatology, key uncertainties remain regarding Holocene climate variability in the Southern Hemisphere, particularly concerning the evolution of the position and intensity of the Southern Westerly Winds (SWW) and their influence on high mountain cryospheric systems. The Subtropical Andes of Chile (30–35°S), located near the northern margin of SWW influence, offer an exceptional geomorphic record derived from glacial and periglacial ice in response to past climatic changes, and therefore suitable for reconstructing Holocene SWW variability.

Well-preserved glacial landforms, such as moraines, have been widely used to reconstruct past periods of increased moisture (e.g. Aguilar et al., 2022; Fernández-Navarro et al., 2023, 2024; García et al., 2024; Sagredo et al., 2017; Zech et al., 2017). In parallel, recent inventories show that the Subtropical Andes of Chile and Argentina host the most extensive periglacial belt in the Southern Hemisphere (Barcaza et al., 2017; DGA, 2022; Masiokas et al., 2020). Rock glaciers, indicative of sustained cold-ground and relatively arid conditions (Azócar & Brenning, 2010), therefore represent a major but still underutilized paleoclimatic archive. Although recent studies have demonstrated the potential of cosmogenic exposure dating of rock glaciers for paleoclimate reconstruction (e.g. Amschwand et al., 2021), this approach has remained unexplored in the Subtropical Andes until now.

Although glacial and periglacial landforms commonly coexist within the same catchments in the Subtropical Andes of Chile (e.g., Aguilar et al., 2022; Carraha et al., 2024), their temporal and morphostratigraphic relationships remain poorly constrained. Consequently, the timing and climatic drivers of glacial and periglacial phases are still mostly unknown (García et al., 2024; Jones et al., 2019), limiting our understanding of the Holocene paleoclimate and its cause. Here we present new 10Be cosmogenic exposure ages from moraines and surface blocks on multi-lobate rock glaciers in the Piedra Valley (30°S) to help constrain the timing and extent of periglaciaton of this valley after the LGM and into the Holocene. This combined glacial–periglacial chronological framework allows us to explore the timing of climatically controlled cryospheric response during the Holocene and their potential relationship with regional hydroclimatic variability. Our results contribute to a better understanding of cryosphere–climate interactions in mid-latitude mountain environments and provide new insights to test proposed hypothesis regarding glacial-periglacial transition at the end of the last ice age, as well as Holocene climate change in the subtropical southern latitudes.

How to cite: Carraha, J., García, J. L., Fernández-Navarro, H., and Amschwand, D.: Holocene climate variability as reconstructed from 10Be dated glacial and periglacial phases in the Subtropical Andes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5879, https://doi.org/10.5194/egusphere-egu26-5879, 2026.

Climate reconstructions across Quaternary glacial cycles are limited in the southern mid-latitudes by a scarcity of terrestrial records. The Falkland Islands (~51°S) offer a key location for addressing this gap. Falklands block streams or ‘stone runs’ are among the most striking and enigmatic landforms on Earth but, despite over a century of study, their origin, and the role of Quaternary climate change, remains debated. We present new constraints on stone run formation using transects of cosmogenic Be-10 and Al-26 measurements. Twenty-six dual-isotopic exposure ages reveal altitudinal patterns that test two competing models: (1) formation during warm, tropical Tertiary conditions, with minimal Quaternary modification; or (2) production and transport under intensely cold, periglacial conditions entirely within the Quaternary. Our results also inform lingering questions about glacier extent and associated climate reconstructions. Falklands stone runs are arguably the most extensive and best-developed blockfield landscapes globally, providing an ideal testbed for examining formation. Our findings advance understanding of long-term blockfield evolution in unglaciated terrain, with implications for similar landscapes worldwide.

How to cite: Darvill, C. and Bentley, M.: Testing models of Falkland Islands Stone Run formation using cosmogenic nuclide exposure dating, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7140, https://doi.org/10.5194/egusphere-egu26-7140, 2026.

EGU26-10579 | ECS | Posters on site | GM9.1

Luminescence dating and 3D modelling of a Mid Pleistocene inner-alpine alluvial-talus succession 

Marei Drexler, Diethard Sanders, and Michael C. Meyer

Sedimentary archives from inner-Alpine settings predating the Last Glacial Maximum (LGM) are rare due to the strong erosional impact of LGM glaciers on these landscapes. In the Eastern Alps, a key site for reconstructing pre-LGM inner-Alpine environmental conditions is located near Innsbruck (Austria): the so-called Höttinger Breccia. This >1300m -thick sedimentary succession consists of basal lodgement till overlain by a thick sequence of alluvial to talus-slope deposits with intercalated aeolian and lacustrine sediments, capped by LGM moraine. Over a century ago, this succession also provided some of the first evidence for the multiple, cyclical nature of the ice ages.

Despite the significance of this site for reconstructing pre-LGM inner-Alpine environmental conditions, chronological constraints on these sediments remain limited. Previous optically stimulated luminescence (OSL) dating of quartz provided only minimum age estimates for the Höttinger Breccia because the quartz signals approached saturation. To overcome this limitation, this study applies infrared-stimulated luminescence (IRSL) dating to feldspar, as the IRSL signal saturates at much higher doses than the quartz OSL signal, thereby enabling dating further back in time. We exploit a range of post-IR IRSL (pIRIR) feldspar signals at stimulation temperatures from 110°C to 290°C to systematically investigate feldspar-related issues of anomalous fading and partial bleaching. We (i) present an optimized dating protocol that identifies the IRSL signal providing the best trade-off between signal stability and bleachability; (ii) report preliminary age estimates obtained from samples taken at various stratigraphic depths within the Höttinger Breccia succession; and (iii) integrate these age estimates into a 3D model of the sedimentary succession.

This combined chronological and spatial framework provides a basis for reconstructing Mid Pleistocene paleoenvironmental conditions in an inner-Alpine valley that otherwise preserves almost no geomorphic record of pre-LGM paleoclimate variability.

How to cite: Drexler, M., Sanders, D., and Meyer, M. C.: Luminescence dating and 3D modelling of a Mid Pleistocene inner-alpine alluvial-talus succession, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10579, https://doi.org/10.5194/egusphere-egu26-10579, 2026.

EGU26-11276 | Orals | GM9.1

Constraining decay of the British-Irish Ice Sheet on Lundy, Celtic Sea, during the Last Glacial Cycle  

David Fink, Phil Hughes, Chris Rolfe, Mark Bateman, Anthony Brown, and Krista Simon

Much has improved about the glacial history of the British-Irish Ice Sheet (BIIS) during the Last Glacial Cycle (MIS 5d) thanks to rich data sets generated by the BRITICE Project.  However, the south-west sector, between the Celtic Sea and Bristol Channel, is challenging because it is largely secured by marine evidence. However, a glacial landscape, preserved on the granitic island of Lundy, exhibits clear evidence of glacial over-printing with remnant transported glacial boulders, glacially-eroded bedrock surfaces, ice scoured tor stumps and erratic gravels. Lundy marks the intersection of ice flow across the eastern boundary of the Celtic Sea and southern extent of the Welsh Ice Cap at the Bristol Channel.  The Celtic Sea transported one of the largest BIIS ice streams and thus has significant implications for understanding rapid deglaciation of large  ice-sheets. Together with the Isles of Scilly, further south by ~125 km, both locations are strategically placed to pin down the southern extent of the history of the BIIS  and answer the question – when during the Last Glacial Cycle did the BIIS overtop Lundy and if so,  did it extend up through the Bristol Channel during the global LGM 27-23 ka yrs ago.  Previous exposure ages ranging from 30-50 kyrs, from Lundy (Rolfe, 2012), notably on bedrock, point to a pre-MIS 3 glaciation (most likely MIS 4) ruling out the conclusion that LGM ice reached Lundy. Given that there is strong evidence (OSL and 10Be dating) for Scilly to have been glaciated during the LGM (Smedley et al 2017), which is also supported by BIIS modelling, debate surrounds assigning Lundy 10Be data to true exposure ages (Carr, 2017). The relatively large age spread possibly resulting from cosmogenic inheritance/erosional irregularities and pegmatite/beryl presence in Lundy granite (Mclintock, 1912) may complicate the interpretation of the exposure ages. 

We have re-visited Lundy and collected 11 new  samples comprising erratic boulders perched on polished bedrock, tor stumps and tops. The tor stumps (tops) would have been the least (most) persistent to preservation of inherited nuclides resetting . The new10Be exposure ages when compared to bedrock ages from Rolfe (2012) should confirm whether the timing of BIIS retreat at Lundy was before or during the LGM. Two OSL samples from cover sands over gravel will provide independent age control.


An interesting aspect of Lundy granite is the presence of beryl, topaz and other insoluble minerals (ie tourmaline). This required considerable care to quantify the intrinsic 9Be concentration. For example, in 3 quartz samples there was sufficient native 9Be to warrant zero addition of 9Be carrier.  Not including a native 9Be contribution would underestimate exposure ages. However, the leaching of meteoric 10Be from these insoluble minerals during quartz dissolution is more of a concern and would result in over estimating exposure ages (Corbett, 2023). The new ages and impact of Lundy granite chemistry for cosmogenic dating will be represented.

Rolfe, QSR, v43, 2012
Carr,  Proc. Geol. Assoc., v128, 2017
Mclintock, Mineral. Magazine, v16, 1912
Smedley, JQS, v32, 2017
Corbett, QG, v73, 2023

How to cite: Fink, D., Hughes, P., Rolfe, C., Bateman, M., Brown, A., and Simon, K.: Constraining decay of the British-Irish Ice Sheet on Lundy, Celtic Sea, during the Last Glacial Cycle , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11276, https://doi.org/10.5194/egusphere-egu26-11276, 2026.

EGU26-11795 | Orals | GM9.1

Persistent Surface Thermal Signatures Following Ice-Patch Ablation in the Scottish Highlands  

Emma Belhadfa, Barbara Katarzyna Francik, Carla Verónica Fuenteslópez, and Sofya Lebedeva

Present-day periglacial landscapes in mid-latitude mountain regions provide critical analogues for understanding both past cryospheric change and future responses of high-latitude systems to ongoing global warming trends. In the Scottish Highlands, long-lived seasonal ice patches have undergone increasingly frequent and extensive melt events in recent decades, reflecting broader patterns of cryosphere retreat documented across alpine and Arctic environments12. These rapidly changing features offer a testbed for examining how ice-ground interactions evolve during and after ice loss, and how their geomorphological and thermal signatures persist within the landscape34. 

During the Oxford University Foundations Expedition to the Cairngorms, Scotland in August 2025, we conducted a grid-based thermal imaging survey of a recently ablated ice patch hollow called the Sphinx to investigate post-melt surface thermal behavior5. Thermal data was collected using a lightweight handheld infrared camera (HIKMICRO E01), enabling systematic acquisition of high-density surface temperature measurements across the former ice basin, its marginal slopes, meltwater channels, and adjacent control surfaces. Field observations, GPS locations, shading context, and surface characteristics were recorded alongside thermal measurements to support interpretations. 

Measurements demonstrated that, within the historical ice patch hollow, the ground temperature averaged 11.52°C ± 0.60°C, 11.88°C ± 1.85°C colder than the adjacent terrain and 7.68°C ± 1.21°C colder than the ambient air temperature at the time of measurement. Hence, we found that coherent thermal anomalies persist following ice loss, which may reflect the former presence, thickness distribution, and melt history of the ice patch. A mosaic reconstruction of the thermal images demonstrates a clear thermal boundary coincident with the historical ice patch, indicating persistently lower surface temperatures relative to surrounding terrain despite the absence of surface ice. 

By combining field-based thermal imaging with geomorphological context, this study demonstrates how present-day periglacial processes in a mid-latitude mountain setting can inform reconstructions of recent cryosphere change and provide analogues for future high-latitude warming scenarios. The Scotland campaign also serves as a methodological testbed for transferable thermal survey strategies applicable across cold-region environments. The expedition team aims to further explore this methodology in Western Greenland in summer 2026.  

How to cite: Belhadfa, E., Francik, B. K., Fuenteslópez, C. V., and Lebedeva, S.: Persistent Surface Thermal Signatures Following Ice-Patch Ablation in the Scottish Highlands , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11795, https://doi.org/10.5194/egusphere-egu26-11795, 2026.

EGU26-12165 | Orals | GM9.1

Links between ice dynamics, subglacial hydrology, and sediment flux from glaciers under increased melt conditions 

Ian Delaney, Audrey Margirier, Marjolein Gevers, Matt Jenkin, Tancrède Leger, Ivan Vergara, Julien Seguinot, Guillaume Jouvet, Alan Robert Alexander Aitken, Stuart N. Lane, Frédéric Herman, and Georgina E. King

Warming-driven melt impacts the landscape in glacierized catchments by altering bedrock erosion and the processes that mobilize subglacial sediment, affecting the delivery of sediment to downstream systems. Here, we synthesize insights from sediment export observations, together with numerical modeling experiments that evaluate ice motion, subglacial water flow, and sediment transport as they respond to change hydro-climatic conditions. The synthesis highlights timescale-dependent controls on sediment production, access, and mobilisation processes. During millennial-scale glacial retreat, steeper ice surfaces and warmer basal conditions increase glacier sliding, likely raising potential sediment production rates through bedrock abrasion. At decadal to annual scales, higher melt elevations allow water to access previously stored subglacial material further upglacier from the ice margin, so that sediment export may increase even as ice thins and sediment production rates fall. At event scales, such as during rapid discharge pulses from precipitation events, heatwaves, or floods, can strongly amplify transport capacity because subglacial conduits adjust slowly, causing intense variations in sediment transport capacity. These interacting processes imply that erosion rate estimates depend strongly on the duration of their observational period, potentially biasing observed rates toward pulses or hiatuses. Lastly, we discuss topics where the impact of greater hydro-climatic conditions on glacier erosion and sediment export is less well understood. These include the transport of sediment from ice sheets, along with the export of large sediment sizes as bedload. Finally, we outline how emerging in-situ sensing, novel geochronology, and next-generation models can better link climate forcing to sediment flux across timescales.

How to cite: Delaney, I., Margirier, A., Gevers, M., Jenkin, M., Leger, T., Vergara, I., Seguinot, J., Jouvet, G., Aitken, A. R. A., Lane, S. N., Herman, F., and King, G. E.: Links between ice dynamics, subglacial hydrology, and sediment flux from glaciers under increased melt conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12165, https://doi.org/10.5194/egusphere-egu26-12165, 2026.

EGU26-13525 | ECS | Orals | GM9.1

Tracer characterization of rock glaciers spring waters in the Eastern Italian Alps 

Enrico Marin, Luca Carturan, Chiara Marchina, Barbara Casentini, Nicolas Guyennon, Laura Marziali, Simona Musazzi, Roberto Seppi, Matteo Zumiani, Stefano Brighenti, Nicola Colombo, Franco Salerno, and Giulia Zuecco

The rapid melting of alpine glaciers is expected to make subsurface ice, including that stored in periglacial formations like rock glaciers (RGs), an important shallow groundwater source for the downstream areas. However, many open questions remain about the ice volume in RGs, its melting rates, hydrological importance, and the quality of water flowing from RGs. This study aims to: i) characterize the geochemistry of RG springs, and ii) assess the variability of environmental tracers in spring waters downstream of RGs with different degree of activity.

We studied springs from intact (ice-embedding) and relict (without ice) RGs, as well as reference springs not influenced by RGs, in six mountain catchments of the Eastern Italian Alps. Sampling campaigns were carried out during two years with different snow and hydrometeorological conditions. While the hydrologic year 2023/2024 was characterized by higher snow cover accumulation and duration, the year 2024/2025 had a shorter accumulation season and most catchments were snow free already in June.

During summer 2024 and 2025, from late June to late September, we conducted sampling campaigns to measure spring water temperature, electrical conductivity (EC), pH, and collect water samples for analyzing stable isotopes of hydrogen and oxygen, major ions, and trace elements. We used automatic samplers to collect samples every 48 hours from one intact RG spring and one relict RG spring to study the temporal dynamics of different tracers.

Springs downstream of relict RGs exhibited lower EC than those from intact RGs. A seasonal isotopic enrichment was observed, likely due to decreasing snowmelt contribution. This seasonal enrichment was more pronounced at higher elevations. Intact RG springs had higher EC and sulphate concentrations compared to relict RGs and reference springs, especially in late summer (September) and in areas underlain by acidic metamorphic rocks (micashists). Water samples collected in 2025 from intact RG springs exhibited higher EC and ion concentrations than those collected in 2024. This contrast underscores the role of seasonal snow and snowmelt in the dilution of solutes released in high-elevation areas, where subsurface ice is likely present.

These initial findings reveal significant geochemical differences between springs from intact RGs and those from relict RGs or reference sites. At some intact RG springs nichel, manganese and sulphate concentrations are not suitable for drinking water, suggesting potential issues for human consumption.

These preliminary results contribute to the limited knowledge of RGs spring water chemistry, stimulating further investigation also including biogeochemical processes eventually involved in the rock-water interface.

This study was carried out within the project PRIN 2022 “SUBSURFICE – Ecohydrological and environmental significance of subsurface ice in alpine catchments” (code no. 2022AL7WKC, CUP: C53D23002020006), which received funding from the European Union NRRP (Mission 4, Component 2, Investment 1.1, D.D. 104 2/2/2022).

How to cite: Marin, E., Carturan, L., Marchina, C., Casentini, B., Guyennon, N., Marziali, L., Musazzi, S., Seppi, R., Zumiani, M., Brighenti, S., Colombo, N., Salerno, F., and Zuecco, G.: Tracer characterization of rock glaciers spring waters in the Eastern Italian Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13525, https://doi.org/10.5194/egusphere-egu26-13525, 2026.

EGU26-15168 | Posters on site | GM9.1

Distribution of supraglacial landslides in the Southern Andes 

Marek Ewertowski and Aleksandra Tomczyk

Supraglacial landslides constitute an important component of glacier–landscape interactions, with the potential to influence glacier dynamics, mass balance, surface evolution, and sediment transport. From a geomorphological perspective, they contribute to the formation of large, anomalously positioned moraines and may, in some cases, facilitate the transition from glacier ice to rock glaciers. However, the glaciological and geomorphological significance of supraglacial landslides is highly variable and depends on landslide geometry, position relative to glacier accumulation and ablation zones, event timing, and the potential for long-term preservation of deposits.

This study investigates the spatial distribution and timing of large supraglacial landslides (>0.2 km² of deposits) across the Southern Andes. Landslide mapping was conducted using a multi-stage remote-sensing approach. First, potential supraglacial landslide locations were identified using high-resolution satellite imagery. Second, time series of medium-resolution satellite data (Landsat, ASTER, and Sentinel) were analysed to constrain the timing of individual events by estimating the occurrence window length (OWL), defined as the interval between the most recent image without a visible landslide and the oldest image in which the landslide deposit is observed. Third, morphometric characteristics were derived, and landslide locations were analysed in relation to glacier zones.

A total of 334 potential supraglacial landslides were identified, of which 198 deposits larger than 0.2 km² were detected on more than one satellite image between 1984 and 2025. For 59 of these landslides, sufficient time-series satellite imagery was available to constrain the OWL and thus approximate event timing. The results indicate that supraglacial landslides in the Southern Andes are substantially more frequent than previously recognised. The mapped inventory and timing constraints provide a basis for future analyses assessing the impact of individual landslides on glacier dynamics and their broader geomorphological significance.

This research was funded by the National Science Centre, Poland, project number 2021/42/E/ST10/00186

How to cite: Ewertowski, M. and Tomczyk, A.: Distribution of supraglacial landslides in the Southern Andes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15168, https://doi.org/10.5194/egusphere-egu26-15168, 2026.

EGU26-16984 | ECS | Posters on site | GM9.1

UAV-based thermal mapping for interpreting geomorphological processes in complex alpine environments 

Leona Repnik, Francesco Comiti, Mattia Gianini, Anne-Laure Argentin, Felix Pitscheider, and Stuart Lane

As a result of climate change, temperatures in the European Alps are rising twice as fast compared to the global average, leading to unprecedented glacier retreat. Deglaciating alpine landscapes are considered extremely dynamic, evolving rapidly over space and time. One of the legacies of glacial activity is buried ice, also known as legacy or dead ice, describing ice that survives in the proglacial area for years to decades after glaciers retreat due to isolation from solar radiation and thermal effects by a sediment cover. Buried ice plays an important role in alpine basins, for instance, by providing long-term water storage. It is also likely to be an important influence on geomorphic processes, such as erosion. Quantification of erosion and deposition patterns from DEMs of difference (DoDs) may be problematic if DoDs do not distinguish geomorphic change from buried ice melt out. Such distinction is commonly omitted in studies, as ground-based geophysical measurements (e.g. Electrical Resistance Tomography, ERT) may need to be applied, extremely difficult given the challenges associated with accessing steep alpine terrain and the spatially extensive areas that may need to be measured. The extent of buried ice is therefore likely to be poorly estimated.

Satellite-based thermal remote sensing may provide a solution to this problem. Indeed, as an example, Interferometric SAR may be used to detect to a very high vertical precision the surface changes that suggest buried ice. However, the spatial resolution of such data may be inefficient when the surface changes are complex. Recent developments in drones and thermal sensors include compact drones with high quality thermal sensors, such as the DJI Mavic 3T. Drones have the benefit of (1) providing a higher spatial resolution compared to satellite thermal remote sensing, and (2) covering larger areas, compared to existing methods of buried ice detection, such as ERT.

In this research, a thermal drone was tested to identify buried ice in the Turtmann basin, a rapidly deglaciating Alpine valley in the Canton of Valais (southwestern Switzerland). Areas known to contain buried ice were surveyed. The assessment of the thermal images showed high coherence between cold patches on the images with known presence of buried ice.

This study highlights the potential for thermal drones in assessing and monitoring geomorphological processes in deglaciating environments, with a specific focus on buried ice. The results provide guidelines on equipment, survey design and execution, as well as data analysis for the use of thermal drones in alpine environments. Future research could focus on identifying approaches for validating the method for surveying areas with no prior knowledge on buried ice. There is a huge potential for the use of thermal drones that is yet to be explored.

How to cite: Repnik, L., Comiti, F., Gianini, M., Argentin, A.-L., Pitscheider, F., and Lane, S.: UAV-based thermal mapping for interpreting geomorphological processes in complex alpine environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16984, https://doi.org/10.5194/egusphere-egu26-16984, 2026.

EGU26-17096 | ECS | Posters on site | GM9.1

The evolution and insulation effect of two recent rockfalls on the Höllentalferner glacier in the Bavarian Alps: A multi-temporal analysis of volume and morphology using LiDAR and UAV data. 

Till Kohlhage, Toni Himmelstoss, Wilfried Hagg, Manuel Stark, Tobias Heckmann, and Florian Haas

In the context of ongoing glacier retreat and slope destabilisation, rockfalls in high-alpine cirque headwalls are becoming increasingly relevant and constitute an integral component of paraglacial process chains. 

On the Höllentalferner (Wetterstein Mountains, Bavarian Alps), two prominent rockfall events occurred in recent years (2016 and 2024), depositing large amounts of debris onto the glacier surface and forming distinct supraglacial debris bodies. The aim of this study is a quantitative assessment of both events focusing on (i) quantifying the rockfall volumes using multi-temporal surface reconstructions and DoD-based estimates, (ii) assessing how supraglacial debris cover modifies glacier ablation by comparing bare-ice melt with melt beneath debris (i.e., differential ablation), and (iii) characterizing the spatio-temporal evolution of debris-body morphology (extent, thickness and internal redistribution) across consecutive observation epochs.

Methodologically, a multi-temporal DEM-of-Difference (DoD) approach is applied that combines, co-registers, and differences UAV/aerial-image-based SfM photogrammetry with airborne laser scanning (ALS) datasets. For this purpose, RTK-UAV surveys (2023 and 2025) are processed photogrammetrically into point clouds, DEMs and orthomosaics. The DEMs are aligned to stable terrain before DoDs are used to quantify elevation and volume changes.

First results indicate that volume estimates strongly depend on the chosen method: for the 2016 rockfall, estimates of approx. 10,410 m³ (extrapolation from bare-ice melt) and 15,510 m³ (Topo-to-Raster interpolation) are obtained, contrasted by a detachment volume of 5,206 m³. Interpolation-based DoD analyses yield epoch-specific volumes on the order of 19,443–31,519 m³, largely driven by differential ablation between debris-covered and adjacent bare-ice areas (and associated changes in the surrounding glacier surface). For the 2024 rockfall, current estimates amount to 20,171 m³ (extrapolation) and 10,128 m³ (detachment volume). Comparing bare-ice melt with melt beneath debris for the 2016 event indicates a pronounced insulating effect: between 2016 and 2018 (extrapolated), bare ice lowered by 4.3 m, whereas the debris-covered area lowered by only 0.8 m (differential ablation −3.5 m).

The findings highlight (i) the need for a multi-method framework to robustly constrain volumes and associated uncertainties, (ii) the key role of debris-driven melt/settlement processes for interpreting DoD signals on debris-covered glacier surfaces, and (iii) the potential of rockfalls deposits to locally delay glacier melt by supplying insulating debris.

How to cite: Kohlhage, T., Himmelstoss, T., Hagg, W., Stark, M., Heckmann, T., and Haas, F.: The evolution and insulation effect of two recent rockfalls on the Höllentalferner glacier in the Bavarian Alps: A multi-temporal analysis of volume and morphology using LiDAR and UAV data., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17096, https://doi.org/10.5194/egusphere-egu26-17096, 2026.

EGU26-18716 | ECS | Posters on site | GM9.1

Mapping crevasse-squeeze ridges- defining characteristics for improved understanding and identification of these landforms 

Anna Ranger, Brice Rea, Matteo Spagnolo, Bartosz Kurjanski, Andrew Newton, Danni Pearce, and Harold Lovell

Crevasse squeeze ridges (CSRs) are landforms indicative of glacier surging and ice stream shut down. They form during fast ice flow, when high basal water pressures and extensional ice flow cause hydrofracturing in the base of the glacier and subsequent squeezing/injection of sediment into basal crevasses. When the fast ice flow phase ends, ice stagnates and down wasting of the ice surface occurs. If lateral support is maintained the sediment ridges are preserved as the glacier passively retreats. Geometries of these ridge networks can thus provide insights into subglacial conditions during phases of fast ice flow. This is important because the rapid movement of ice from areas of accumulation to ablation zones, during fast ice flow phases, exposes a greater area of ice to melting having long term impacts on the mass balance of these glaciers.

CSR characteristics have been inconsistently reported in the literature and in some cases have been misidentified. Here we present the first global dataset combining CSR information mined from the literature with new mapping and use this to define CSR characteristics in both surging and ice stream contexts as well as in terrestrial and marine settings. Using ArcGIS Pro, we map ridges from high resolution aerial imagery and digital elevation models, and extract metrics on ridge lengths, network density, and orientations in relation to ice flow direction. CSRs have been mapped at modern surge-type glaciers in Iceland and Svalbard, and in palaeo-landscapes in central Canada, the British Isles, and Northern Europe related to ice stream shutdown. Furthermore, we categorise the data into marine and terrestrial environments because CSRs are often better preserved in marine settings, due to the action of subaerial and meltwater erosional processes occurring on land.

This new dataset provides a representative understanding of CSR morphologies to allow better identification of the landform in the future, which will help to understand subglacial processes beneath fast-flowing ice masses. Understanding basal conditions in any glacial system is challenging due to the difficulties of acquiring direct measurements at the base of the glacier. CSRs represent these basal conditions and can therefore provide insights.

How to cite: Ranger, A., Rea, B., Spagnolo, M., Kurjanski, B., Newton, A., Pearce, D., and Lovell, H.: Mapping crevasse-squeeze ridges- defining characteristics for improved understanding and identification of these landforms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18716, https://doi.org/10.5194/egusphere-egu26-18716, 2026.

EGU26-19000 | Orals | GM9.1

Characteristics and evolution of ice-debris complexes in deglaciating mountain environments investigated by remote sensing and in-situ surveys 

Tobias Bolch, Ella Wood, Zhangyu Sun, Daniel Falaschi, Atanu Bhattacharya, Benjamin Robson, Vassiliy Kapitsa, and Lothar Schrott

Ice-debris complexes are compound landforms, including glaciers, debris-covered glaciers and rock glaciers, that exist at the interface between the glacial, periglacial and paraglacial realms. These landforms are common in many mountain ranges on Earth, but the hydrological and geomorphological role of these ice-debris complexes in the context of deglaciating mountain environments is still not well understood. This is in part due to challenges arising from their position bridging different disciplines, categorisations, and research methodologies.

In this talk we present findings from our work based on in-situ investigations (including ground penetrating radar [GPR] and electrical resistivity tomography [ERT)] measurements) and multi-temporal high resolution remotely-sensed image analysis (based on historical aerial images, declassified Corona KH 4 images and contemporary data such as Pléiades satellite images) conducted on selected ice-debris complexes in the Tien Shan, Central Asia and further comparison with examples from the Pamirs, Andes and the European Alps.

Results show that the response of debris-covered glaciers, glacier-connected rock glaciers and talus-connected rock glaciers to climate change strongly differs, partly due to the different sources and amount of debris and ice inputs. The presence and distribution of massive ice varies across geomorphic units and is linked to the types of glacial-periglacial interaction. For example, we identify a significant amount of ice buried beneath debris cover in glacier forefields in transition to rock glaciers and in the glacier-connected rock glacier parts. Debris supply is important in controlling the development and flow activity of the morphological units. The response of rock glaciers to climate change is heterogenous with overall increasing velocities and on average only slight surface elevation changes. Glacier-connected rock glaciers flow on average faster than talus-connected rock glaciers. DEM differencing reveals slight increases in surface elevation at the rock glacier termini while debris-covered glaciers show on average a clear signal of surface lowering and decreasing velocities. This highlights the importance of understanding of the debris-sources and the interplay between the glacial and periglacial components of the ice-debris complexes when considering the hydrological and geomorphic role of these landforms.

How to cite: Bolch, T., Wood, E., Sun, Z., Falaschi, D., Bhattacharya, A., Robson, B., Kapitsa, V., and Schrott, L.: Characteristics and evolution of ice-debris complexes in deglaciating mountain environments investigated by remote sensing and in-situ surveys, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19000, https://doi.org/10.5194/egusphere-egu26-19000, 2026.

EGU26-19657 | ECS | Posters on site | GM9.1

Long-term monitoring of rock glacier displacement - adaptation of methodology in response to new challenges 

Anne Hartig, Martin Stocker-Waldhuber, Bernd Seiser, Lea Hartl, and Andrea Fischer

In recent years, in situ monitoring of rock glacier displacement has become more challenging. Unstable slopes, higher probability of gravitational movement due to destabilization processes and rock fall are negatively impacting the accessibility of research sites. To maintain long-term time series, current monitoring techniques need to be adapted.

One example of a research site affected by this is Äußeres Hochebenkar rock glacier (46°50'0"N, 11°0'30"E, Ötztal Alps, Austria). The rock glacier has been subject to velocity measurements since 1938, making it one of the longest time series worldwide. Differential Global Navigation Satellite System (dGNSS) measurements are carried out since 2007. Aside minor data gaps, velocity data have been available at annual resolution since 1997 from four cross sections and a longitudinal profile. Each profile consists of 6 to 12 individual block positions.

For the majority of the time series, the flow velocity was hardly more than 1 m/a on average. Since 2018, an exponential increase of rock glacier motion has been observed in the lowest section, showing the destabilization of this part of the rock glacier. During the last three years, maximum displacement values at individual blocks increased from 20 m/a to almost 50 m/a in 2024 and 75 m/a in 2025.

Accessing the block profiles in the destabilized section to carry out dGNESS measurements has become challenging. To ensure the continuity of the time-series, UAV surveys have been incorporated in the monitoring program. In 2024 and 2025, multitemporal optical imagery was acquired in addition to dGNSS dataHigh-resolution othormosaics and digital elevation models were derived from the UAV imagery using Structure-from-Motion (SfM) photogrammetry techniques. This enables the calculation of spatially distributed displacement vectors over the whole rock glacier from multitemporal hillshades using image correlation algorithms and provides alternative observations of block displacement.

We present the displacement rates for the years 2024 and 2025 using the most recent workflow, comparing displacement rates from dGNSS measurements with those derived from mapping on high-resolution orthomosaics and image correlation of multitemporal hillshades. We show how dGNSS displacement can be complemented by and compared to UAV-based methods. We try to address the opportunities and uncertainties lying within these approaches for mountain landforms that are reacting quickly to environmental changes, assuming that more and more comparable cases will arise under current and future climatic conditions in high mountain regions.

How to cite: Hartig, A., Stocker-Waldhuber, M., Seiser, B., Hartl, L., and Fischer, A.: Long-term monitoring of rock glacier displacement - adaptation of methodology in response to new challenges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19657, https://doi.org/10.5194/egusphere-egu26-19657, 2026.

Frost weathering is a fundamental process controlling bedrock fracturing and rockfall activity in alpine environments, and its understanding requires evaluating the influence of snow cover on the thermal distribution at the bedrock surface (Matsuoka and Murton, 2008; Eckerstorfer et al., 2012; Haberkorn et al., 2017). In the Japanese Alps, characterized by heavy rainfall and snowfall, rock temperature data remain limited compared to the European Alps, which lie in the same mid-latitude zone as Japan. Moreover, long-term monitoring in the Japanese Alps has been confined to areas with relatively low snow accumulation (e.g., Matsuoka, 2019). In this study, we aim to clarify the conditions favorable for frost cracking in the heavy snow region by monitoring rock temperature, maximum snow depth, and snow-cover duration under various snow conditions on Mt. Hakuba (2,932 m a.s.l.) and Mt. Shakushi (2,812 m a.s.l.), located in the northern Japanese Alps.

From October 2021 to September 2025, we continuously monitored rock temperatures at depths mainly of 2 cm, 20 cm, and 40 cm, and locally down to a maximum depth of 120 cm. In addition, aerial surveys were conducted using a Cessna aircraft and UAVs. 3D point cloud models of rock slopes for different seasons were generated from aerial images using SfM/MVS analysis. Maximum snow depth at each sensor location was obtained from point cloud distance calculations between models representing the maximum snow accumulation and the snow-free period when bedrock is exposed. From the rock temperature data, several indices related to frost cracking were calculated, including annual freeze–thaw cycles (Matsuoka, 2002), freezing degree days, the duration of temperatures within the frost cracking window, and thermal gradient conditions (Kellerer-Pirklbauer, 2017). These indices were compared with interannual variations in snow depth and snow-cover duration.

In the results, snow-cover duration varied substantially between years, resulting in pronounced differences in frost cracking indices at each site. In addition, the height of snow cornices formed along ridges was greater than in heavy snow years, even when the overall snow cover duration was short, highlighting strong spatial heterogeneity in snow conditions near ridges. Although longer snow covers tended to raise winter rock temperatures, fractured bedrock sites showed lower temperatures and high freezing degree days. Future changes in frost cracking indices were calculated for each site based on various air-temperature warming scenarios, revealing markedly different trends depending on the scenario. These findings provide valuable insights for assessing present and future frost cracking potential in snow-rich alpine regions of Japan.

How to cite: Sugiyama, H. and Narama, C.: Four-year monitoring of rock temperature and snow conditions relevant to frost weathering in the northern Japanese Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21081, https://doi.org/10.5194/egusphere-egu26-21081, 2026.

The link between rock glacier velocity and climatic forcing is well established in permafrost research, especially for rock glaciers. This understanding underpins the inclusion of rock glacier velocity as an associated parameter of the Essential Climate Variable “Permafrost” within the Global Climate Observing System since October 2022. In this context, the rock glacier velocity (commonly abbreviated as RGV) is defined as a spatially averaged interannual horizontal velocity time series related to a RG unit or a part of it. However, RGV does not invariably track climatic forcing in a simple, linear manner, which can obscure the climatic signal. In this study, we combine primarily multi-decadal RGV monitoring with long-term observations of ground surface and near-surface temperatures, as well as spring water temperatures, at two sites in the Hohe Tauern, Austrian Alps: the Dösen rock glacier (DOE) and the Hinteres Langtalkar rock glacier (HLK). Both are well-developed, typical alpine rock glaciers. Each features a dominant rock glacier spring that drains runoff from the landform and its contributing hydrologal catchment. Annual in-situ geodetic surveys began in 1995 (DOE) and 1999 (HLK). Ground surface and near-surface temperatures, along with several meteorological variables, have been monitored using miniature temperature loggers and standard meteorological sensors since 2006 at both sites. Spring water temperature monitoring started in 2016 at DOE and 2017 at HLK. Our results indicate a clear relationship, in part, between RGV and temperature (air, ground, water). However, this relationship weakens or disappears where geodetic points are not, or are only partially, representative of permafrost creep. Moreover, summer spring-water temperatures can be damped by heat exchange with internal ice, such that melt of the ice component buffers water peak temperatures. These findings underscore the importance of parallel, co-located monitoring of ground, water, and air temperatures (and other climatic parameters), alongside carefully designed geodetic sampling that targets zones of active permafrost creep.

How to cite: Kellerer-Pirklbauer, A. and Kaufmann, V.: Velocities of rock glaciers and their surface, near surface and hydrothermal regimes in the Austrian Alps: Clear signs of climate change?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21296, https://doi.org/10.5194/egusphere-egu26-21296, 2026.

CR5 – Snow and ice: properties, processes, hazards

Seasonal snowpack is one of the primary sources of freshwater for rivers in the Indian Himalaya. It plays a vital role in regional hydrology, climate variability, and water resource management. To understand these processes and their impact on the community, spatial and temporal monitoring of snow is essential. Snow depth is a key parameter for monitoring snow. However, in the Himalayas, due to accessibility challenges and logistical constraints,  limited snow depth observations are available. To address this gap and estimate snow depth at high spatial and temporal resolution, we develop a model using polarimetric parameters derived from Sentinel-1 SAR data, topographic and auxiliary data, integrated with field-based observations in the European Alps and Grand Mesa, USA. Field observations are filtered to match the Sentinel-1 pass, ensuring consistency between field-based observations and satellite acquisition. Our model employs topographic data (e.g., elevation, slope, and aspect) from the Copernicus 30 m digital elevation model, auxiliary parameters (such as day of the season (DoS)), Forest cover fraction from MODIS, and Sentinel-1 SAR-based polarimetric parameters (cross-ratio, entropy, Stokes parameters, alpha), ensuring a topographically dependent snow depth distribution. Sensitivity analysis is performed using SHAP (SHapley Additive Explanations) to identify the most critical parameters for estimating snow depth. The model shows a Mean Absolute Error (MAE) of 0.04m, a root mean square error (RMSE) of 0.15m, with a test R-squared (R2) of 0.95 and a cross-validation correlation coefficient (R) of 0.98 in the European Alps. We transfer the model to the mountains in the Chandra Bagha basin (33°01′N°, 76°40′E) of the Indian Himalayas. Our transferred model highlights the potential of estimating snow depth in data-scarce regions while resolving the spatial and temporal details. 

How to cite: Sharma, P. and Vijay, S.: Snow depth estimation model calibration and validation for high-altitude glacier valleys in the Indian Himalaya., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-738, https://doi.org/10.5194/egusphere-egu26-738, 2026.

EGU26-951 | ECS | PICO | CR5.1

Two decades of snow pit measurements in Sodankylä, Finland 

Leena Leppänen, Anna Kontu, Henna-Reetta Hannula, Aleksi Rimali, and Heidi Rytkönen

We present a 20-year timeseries of key snow properties measured in Sodankylä, northern Finland. Systematic snow pit observations began in 2006, and the range of measured variables and instruments has expanded substantially over time. Initially, observations included snow depth, stratigraphy, grain size, and temperature, recorded twice per week at a forest opening site. Snow water equivalent (SWE) measurements were added in 2007, density profiles and liquid water content in 2009, and specific surface area (SSA) measurements in 2012. Since 2010, snow pit observations have been conducted once per week.

The monitored locations have varied over the years. A forest opening site was observed from 2006 to 2018, a wetland site from 2009 to 2015 and again from 2019 onward, and a forest site has been included since 2018. Additional snow pits were dug at Lake Orajärvi between 2009 and 2014. Currently, routine observations are carried out at two sites: a wetland and a forest.

The present snow pit protocol includes definition of stratigraphy, a temperature profile measured every 10 cm, and estimation of grain size and grain type, complemented by macrophotography of grain samples from each layer. Density measurements are performed at the surface and at 5 cm vertical intervals using a rectangular cutter. When snow is wet, liquid water content is measured with a WISe instrument at the same heights as the density samples. SSA is measured using InfraSnow for the surface and ice layers, while other layers are measured with IceCube. For thicker layers, IceCube samples are taken every 5 cm. Penetration resistance is measured with SnowScope. Finally, bulk SWE is measured using a snow tube, and snow depth is measured at three points around each pit.

This 20-year dataset provides a unique opportunity to examine long-term changes in snowpack structure and properties, and it illustrates the impacts of a changing climate in snow conditions in northern Finland.

How to cite: Leppänen, L., Kontu, A., Hannula, H.-R., Rimali, A., and Rytkönen, H.: Two decades of snow pit measurements in Sodankylä, Finland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-951, https://doi.org/10.5194/egusphere-egu26-951, 2026.

EGU26-1390 | PICO | CR5.1

A decade of rain-on-snow detection in the Canadian Arctic: Insights from Remote Sensing and Inuit Knowledge 

Alexandre Langlois, Josée-Anne Langlois, Vincent Sasseville, and Cheryl Ann Johnson

Rain-on-snow (ROS) events are increasing across the Arctic as the region warms, altering snow microstructure, creating ice crusts, and impacting wildlife and surface conditions. To better document these events, we combine high-resolution passive microwave data, in situ measurements, climate reanalysis, and Inuit knowledge to assess ROS variability across the Canadian Arctic Archipelago from 1987–2019. Using both fixed and variable winter windows, and validating with meteorological stations, we detect a rise in absolute ROS occurrence, especially along coastal regions. A focused analysis on Banks Island shows significantly greater ROS-affected areas in the fall, with coastal zones experiencing the highest frequency. We find that atmospheric rivers and declining autumn sea ice both contribute to increased ROS occurrence and intensity. By integrating remote sensing with Inuit observations, we improve large-scale ROS detection and understanding of their ecological consequences, particularly for Peary caribou and the communities dependent on them.

How to cite: Langlois, A., Langlois, J.-A., Sasseville, V., and Johnson, C. A.: A decade of rain-on-snow detection in the Canadian Arctic: Insights from Remote Sensing and Inuit Knowledge, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1390, https://doi.org/10.5194/egusphere-egu26-1390, 2026.

EGU26-2816 | PICO | CR5.1

Snow Modelling Locked Pastures from Rain-on-Snow Events in the Arctic 

Érika Boisvert-Vigneault, Melody Sandells, Vincent Vionnet, Nicolas Leroux, Nick Rutter, Alexandre Langlois, and Hannah Bloomfield

Rain-on-snow (ROS) events are an increasingly prevalent Arctic extreme weather phenomenon, driven by accelerated atmospheric warming. These events create ice layers within the snowpack, which can prevent foraging for ungulates like reindeers, caribou and muskoxen and have been linked to catastrophic herd die-offs. Accurately simulating physical consequences of ROS, specifically development of these ice crusts, is therefore critical for assessing wildlife habitat suitability. However, the performance of detailed snow models in high-latitude environments remains inadequately evaluated, particularly their ability to replicate the snowpack stratigraphy following complex meteorological events.

This study investigates the capacity of the snow model Crocus-SVS2 to simulate the impacts of known, major ROS events on the snowpack of Banks Island, Nunavut. We focus on a case study where a documented ROS event was followed by a severe muskoxen mortality event in the winter of 2003-2004. Our methodology forces Crocus-SVS2 with three meteorological reanalysis datasets: the Canadian Surface Reanalysis version 2.1 (CaSR2.1) and 3.1 (CaSR3.1), and ERA5 reanalysis. This multi-forcing approach allows to assess not only the model's physical fidelity but also the sensitivity of the simulations to different weather inputs, thereby evaluating the ability of reanalysis products to represent ROS in the Arctic accurately.

Model outputs are analysed to determine if Crocus-SVS2 can successfully replicate the formation, thickness, and vertical position of observed ice lenses within the snow profile. The primary outcome is a robust evaluation of whether an operational snow model, when driven by the best available meteorological data, can serve as a reliable tool for retrospectively analysing ROS impacts in data-sparse Arctic regions. This research also provides a framework to identify key meteorological conditions that separate minor ROS events from those causing catastrophic ungulate die-offs.

How to cite: Boisvert-Vigneault, É., Sandells, M., Vionnet, V., Leroux, N., Rutter, N., Langlois, A., and Bloomfield, H.: Snow Modelling Locked Pastures from Rain-on-Snow Events in the Arctic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2816, https://doi.org/10.5194/egusphere-egu26-2816, 2026.

EGU26-4478 | ECS | PICO | CR5.1

Development of Percolation Features After a Rain-on-Snow Event in the Southern Taiga  

Anton Komarov and Julienne Stroeve

In this study, we investigate the development of percolation columns in fine-grained snow triggered by the accumulation of liquid precipitation on a cold, dry snowpack during a rain-on-snow (ROS) event in the Southern Taiga. We analyze snow physical properties, stratigraphy, and meteorological conditions before and after the percolation event, documenting changes in snow layering and the formation of percolation columns. Furthermore, we examine how local-scale factors, such as ground surface microtopography and vegetation cover, influence the spatial distribution of these features by comparing snow properties at three adjacent sites with distinctly different surface and vegetation characteristics.

Our results demonstrate that, under certain conditions, percolation columns can form even within fine-grained, low-density snow. Their spatial distribution appears strongly influenced by ground microtopography, with preferential formation between tussocks, while the presence of deciduous vegetation may inhibit their development. Additionally, we discuss the development of preferential flow paths on the adjacent slope that formed simultaneously to the development of percolation columns on flat surfaces and describe the major morphological features we observed. These findings contribute to a deeper understanding of preferential flow in snow and highlight the need to consider localized environmental conditions and evolving climate patterns in future snow hydrology research and hazard forecasting models.

Our observations also provide valuable information for improving the representation of preferential flow processes, which remain a major source of uncertainty in snow models. The distinct vertical icy features associated with percolation columns are also likely to affect radar signal penetration and backscatter, with potential implications for the interpretation of remote sensing observations. Moreover, the fact that such features can be identified from above, for example using drone imagery, offers opportunities for model evaluation and spatial validation under natural conditions.

How to cite: Komarov, A. and Stroeve, J.: Development of Percolation Features After a Rain-on-Snow Event in the Southern Taiga , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4478, https://doi.org/10.5194/egusphere-egu26-4478, 2026.

EGU26-5591 | ECS | PICO | CR5.1

Deriving the evolution of snow specific surface area from water vapor physics at the microstructure scale 

Kevin Fourteau, Anna Braun, Michael Lehning, and Henning Löwe

The specific surface area (SSA) is a crucial parameter to characterize the microstructure of snow. It is one of the main properties controlling the optical and mechanical behavior of snow. Thus, being able to describe the evolution of SSA under the effects of metamorphism is key for detailed numerical snowpack models. This then allows simulating for example the albedo of snow-covered surfaces and its evolution over time. To this end, we propose to derive the law governing the evolution of SSA of snow directly from the physics of water vapor transport at the microstructure scale. We identify the crucial physical parameters for the evolution of the SSA. We show that the evolution of SSA is generally composed of two additive terms: an isothermal contribution and a temperature gradient contribution, each characterized by scalar macroscopic properties relating the evolution of the SSA to the temperature and temperature gradient imposed to the snow. On-going work includes parameterizing these scalar properties in order to obtain a fully-closed and operational law for the evolution of SSA.

How to cite: Fourteau, K., Braun, A., Lehning, M., and Löwe, H.: Deriving the evolution of snow specific surface area from water vapor physics at the microstructure scale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5591, https://doi.org/10.5194/egusphere-egu26-5591, 2026.

EGU26-5841 | ECS | PICO | CR5.1

Emerging contaminants during Arctic Rain-On-Snow events: insights from the 2023-24 Ny-Ålesund campaign 

Azzurra Spagnesi, Stefania Gilardoni, Roberto Salzano, Matteo Feltracco, Beatrice Ulgelmo, Riccardo Maetzke, Francisco Ardini, Marco Grotti, Veronica Coppolaro, Tessa Viglezio, Simonetta Montaguti, Federico Scoto, Andrea Spolaor, Andrea Gambaro, Carlo Barbante, and Elena Barbaro

The Svalbard Archipelago has experienced rapid warming in recent decades, leading to an increased frequency and intensity of Rain-on-Snow (ROS) events. While the physical and ecological impacts of ROS in the Arctic are well documented, their potential role in influencing the atmospheric fate of emerging contaminants remains largely unexplored. This study examines the chemical signature of four ROS events observed during the 2023–24 field campaign in Ny-Ålesund (Kongsfjorden, Svalbard, Norway), with particular attention to the behaviour of emerging pollutants before, during, and after each event. By integrating aerosol and wet deposition measurements with meteorological parameters and air-mass back-trajectory analyses, we assess the capacity of ROS events to act as removal processes for benzothiazole derivatives, tris(2-carboxyethyl)phosphine (TCEP) used as a flame retardant, pesticides, and haloacetic acids. Our results reveal marked variability in contaminant patterns across events, indicating a strong influence of synoptic-scale air mass origins and local meteorological conditions. Diagnostic ratios and inorganic ion tracers further provide insights into potential atmospheric transformation pathways and transport mechanisms. This study presents the first detailed chemical characterisation of aerosols and depositions associated with Rain-on-Snow events, offering a preliminary framework to better understand the interactions between ROS processes and contaminant cycling in a rapidly warming Arctic. This work contributes to ongoing efforts to elucidate atmospheric scavenging mechanisms under changing climate conditions.

How to cite: Spagnesi, A., Gilardoni, S., Salzano, R., Feltracco, M., Ulgelmo, B., Maetzke, R., Ardini, F., Grotti, M., Coppolaro, V., Viglezio, T., Montaguti, S., Scoto, F., Spolaor, A., Gambaro, A., Barbante, C., and Barbaro, E.: Emerging contaminants during Arctic Rain-On-Snow events: insights from the 2023-24 Ny-Ålesund campaign, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5841, https://doi.org/10.5194/egusphere-egu26-5841, 2026.

EGU26-6561 | ECS | PICO | CR5.1

Improvements of a subcanopy snow model conveyed by observations from a mid-altitude alpine site 

Thomas Pauze, Axel Bouchet, Aaron Boone, Matthieu Lafaysse, Mathieu Fructus, Agnès Rivière, Lejeune Yves, and Gouttevin Isabelle

In the Alpine region, forests cover about 2/3 of the ground, yet surface and/or snow models designed for hydrological applications, often represent them in a very coarse way.

In the current study, we present and evaluate new developments in the physics-based ISBA/MEB-Crocus model that enables a detailed representation of snow cover and processes in interaction with an above-lying 1-layer canopy and atmosphere, and with a litter layer on top of the ground. While the canopy representation within this model demonstrated an added value for climate modeling, due to a better representation of snowpack in subarctic regions characterised by boreal forests, ISBA/MEB-Crocus failed to reproduce the observed snowpack at a mid-altitude alpine forest site, systematically overestimating the snowpack in terms of depth and duration.

With a view of correcting for these biases, we use detailed snowpack and meteorological measurements available at the Col de Porte research site in the Chartreuse massif, France, at both open and forested sites. In addition to conventional measures, indirect interception measurements and tree and soil temperatures are recorded.

The use of this dataset enables the improvement of the MEB-Crocus model for alpine forests. This enhancement is achieved through an adaptation of the interception scheme, a revision of the melt parametrization for intercepted snow, and of the unloading scheme. The meteorological forcing is also adapted to align with the top-of-canopy conditions. We demonstrate that these adjustements enable the snowpack model to replicate the observations for the Col de Porte forest site without degrading the results for Artic regions. Furthermore, we characterize the influence of the various parameters employed for the representation of the forest and their physical consistency.

This detailed, point-scale evaluation paves the way for the use of this model for distributed simulations enabling an insight into the role of snow and snow-forest interactions in the hydrological regime of mid-altitude alpine catchments.

How to cite: Pauze, T., Bouchet, A., Boone, A., Lafaysse, M., Fructus, M., Rivière, A., Yves, L., and Isabelle, G.: Improvements of a subcanopy snow model conveyed by observations from a mid-altitude alpine site, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6561, https://doi.org/10.5194/egusphere-egu26-6561, 2026.

EGU26-6663 | ECS | PICO | CR5.1

Changes in Snowmelt Timing and Peak Flow Generation in Non-Regulated Finnish Catchments 

Maedeh Edraki and Ali Torabi Haghighi

Climate change alters precipitation patterns and extends the warm season in Arctic and sub-Arctic regions, with direct consequences for river flow dynamics. Snow Water Equivalent (SWE) provides a critical link between climate forcing and streamflow response, as it represents the portion of the snowpack that is released as runoff. However, temporal analysis of SWE is challenged by the discontinuous nature of observations provided by the Finnish Environment Institute (SYKE). In this study, a degree-day model was used to generate daily SWE time series, which were subsequently corrected using observed data, for four non-regulated Finnish catchments. River flow timing was analyzed relative to snowmelt onset over the period 1982–2024. While no clear trend was identified in the calendar-day occurrence of spring peak discharge, analysis relative to snowmelt onset revealed a consistent shift toward later peak flow, indicating an increasing delay between melt initiation and maximum discharge. Temperature analysis during the snowmelt period showed a significant increasing trend, suggesting warmer melt-season conditions that promote intensified melt but also modify the timing of runoff generation. In addition, precipitation analysis indicated an increasing tendency toward rain-on-snow events, as well as a rising frequency of rainfall occurring between maximum SWE and peak discharge. These results indicate a potential shift from predominantly snowmelt-driven to increasingly rain-driven peak flow.

How to cite: Edraki, M. and Torabi Haghighi, A.: Changes in Snowmelt Timing and Peak Flow Generation in Non-Regulated Finnish Catchments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6663, https://doi.org/10.5194/egusphere-egu26-6663, 2026.

Dry snow microstructure refers to the complex three-dimensional arrangement of ice and air at the sub-millimeter scale. This microstructure undergoes constant shape transformations known as snow metamorphism. These transformations are driven by variations in equilibrium vapor pressure at the ice-air interface, which depend on the local curvature and temperature gradient. A key descriptor of snow microstructure is the specific surface area (SSA), which is the surface area of the ice and air interfaces normalized per ice volume or mass. This metric is commonly used to quantify the average grain size in snowpack models. Moreover, SSA affects important physical properties of the snowpack, including the spectral albedo of the surface and fluid permeability. Consequently, accurately representing SSA evolution in snowpack models is crucial. Overall, snow SSA decays over time, except in specific conditions where SSA increases, such as high temperature gradients. Current descriptions of SSA in snowpack models, such as CROCUS or SNOWPACK, are not fully satisfying, especially they fail to reproduce SSA increase. It restricts the model’s ability to represent processes under high temperature gradients, as typically occurring in Arctic regions. Recent efforts have been made to derive theoretical relations between SSA and microstructural and growth parameters, but have been applied to a limited number of snow evolution experiments.

In this work, we build upon these previous studies and investigate the physical mechanisms driving SSA evolution for numerous dry snow metamorphism scenarios. We re-derive a relationship between the SSA temporal evolution, the local interface growth velocity, and the local mean curvature. To examine the implications of this relation on different snow microstructures, we acquired 20 time series of 3D X-ray tomographic images of dry snow metamorphism at high temporal and spatial resolution during cold-lab experiments. These experiments span a wide range of thermal boundary conditions and initial snow types. Using this data set, we compute local properties on the grain surface, including interface growth velocity, mean curvature, and temperature gradients. Focusing on a subset of experiments, we present SSA evolution for temperature gradients ranging from 10 to 100 K/m. In particular, we investigate the mechanisms responsible for SSA increase at high temperature gradients. We aim to disentangle the respective contributions of local microstructural shape and local temperature gradients to the overall SSA evolution. A more comprehensive understanding of the mechanisms at stake in the SSA evolution will help develop a robust representation of SSA in snowpack models.

How to cite: Dick, O., Calonne, N., and Hagenmuller, P.: Specific surface area evolution during dry snow metamorphism: insights from interface growth velocity computed on 4D tomographic data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7829, https://doi.org/10.5194/egusphere-egu26-7829, 2026.

EGU26-8497 | PICO | CR5.1

Modeling depth hoar snow and its impact on permafrost and greenhouse gas fluxes 

Hotaek Park, Kazuyoshi Suzuki, and Steven Fassnacht

Recent permafrost temperature observations show warming, likely due to the combined impacts of more snow insulation and increased air temperatures. Depth hoar refers to coarse, faceted snow crystals that form near the bottom of the snowpack due to a strong temperature gradient that induces a vapor gradient. The thin and sparse connection between depth hoar crystals results in lower snow density. The depth hoar formed in a snowpack likely enhances permafrost warming during the winter season, and the impact could be sequentially fed back to CO2 fluxes from the permafrost soil during the next growing season. However, little quantitative assessments have been made on the impact of depth hoar on permafrost temperature and the associated feedback to CO2 fluxes. To address this deficiency, we coupled the depth hoar process to the land surface model CHANGE. The model assessed the impact of the depth hoar on permafrost and the associated greenhouse gases, based on two experiments that included or excluded the depth hoar process, over the pan-Arctic scale for the period 1979–2019. The differences between the two experiments illustrated that the depth hoar induced lower snow density and the resultant warmer permafrost temperature was linked to both larger vegetation photosynthesis and decomposition of soil organic carbon. These results strongly suggest that these snow processes improvement should be included in land surface models for better simulations and future projections on the Arctic environmental changes.

How to cite: Park, H., Suzuki, K., and Fassnacht, S.: Modeling depth hoar snow and its impact on permafrost and greenhouse gas fluxes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8497, https://doi.org/10.5194/egusphere-egu26-8497, 2026.

Accurate observation of seasonal snow depth (SD) across spatial scales remains a major challenge in mid-latitude regions, particularly over complex terrain where sub-footprint heterogeneity and scale mismatch strongly affect satellite-based retrievals. Although ICESat-2 has demonstrated high potential for SD estimation in high-latitude regions, its performance in mid-latitude areas is constrained by the limited availability of snow-free digital elevation models (DEMs) with centimeter-level vertical accuracy and by the scarcity of reliable ground-based validation due to ground-track shifting.

To address these challenges, we established a multi-scale “ground-airborne-satellite” synergistic observation framework within a controlled study area in northern Xinjiang, China. To reconcile spatial scale mismatches among the different observational platforms, UAV-LiDAR data were employed as a validated intermediate-scale bridge (RMSE = 6.03 cm against in-situ measurements). Based on this framework, we conducted an error propagation analysis to quantify ICESat-2 SD uncertainty under varying terrain conditions.

Results indicate that ICESat-2 achieves excellent accuracy over flat, open terrain (slope < 5°), with an RMSE of 6.69 cm. In contrast, over complex sub-footprint terrain combining steep slopes and artificial structures, SD deviations increased substantially, ranging from -30 to +60 cm, reflecting the strong influence of sub-footprint terrain heterogeneity on SD retrieval. Across the entire study area, ICESat-2 maintains robust overall performance, yielding a total RMSE of 15.61 cm.

This study demonstrates the feasibility of accurate ICESat-2 SD retrieval in mid-latitude regions and emphasizes the critical influence of sub-footprint terrain complexity on SD uncertainty. The proposed multi-scale observational framework provides a transferable approach for interpreting satellite-derived snow products and for improving the representation of snow processes across scales.

How to cite: zhu, L. and Zheng, L.: Monitoring Snow Depth with ICESat-2 at mid-latitudes: A Synergistic Multi-Scale Framework Integrating Ground-Airborne-Satellite Observations in Northern Xinjiang, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10265, https://doi.org/10.5194/egusphere-egu26-10265, 2026.

EGU26-11937 | PICO | CR5.1 | Highlight

Field Studies of Feldspar-Assisted Snowmaking: Effects on Snow Volume, Density, and Reflectivity 

Albert Verdaguer, Júlia Canet, and Laura Rodríguez

Under most atmospheric conditions, snowfall is triggered by the freezing of supercooled water droplets in clouds through heterogeneous nucleation on airborne particles. Among the most efficient atmospheric ice-nucleating particles, capable of inducing freezing at temperatures only a few degrees below 0 °C, are feldspar minerals. Certain feldspars are known to initiate ice nucleation very efficiently at relatively warm subzero temperatures [1], which has led to their application in snowmaking [2] and controlled freezing processes [3].

In our group, we study the properties of snow produced with the aid of feldspar ice-nucleating particles under real environmental conditions at a Snow Laboratory located in the La Molina ski resort (Spain). In this work, we present results from field studies conducted during the 2022–2023 and 2023–2024 snow seasons. The Snow Lab consists of two technically identical and independent snow guns installed 25 m apart (see Figure a). Snow was produced under varying environmental conditions. In one snow gun, only reservoir water was used, while in the second gun a feldspar powder with high ice-nucleating efficiency [4] was added to the water supply.

The volume and physical properties of the produced snow, including density and reflectivity, were systematically compared between snow generated with and without feldspar additives. Three-dimensional maps of snow volume and physical properties were constructed from a grid of field measurements. The results show that, for the same amount of water, a larger volume of snow is produced when feldspar particles are introduced. In addition, feldspar-assisted snow exhibits lower surface density and higher reflectivity, indicating a modified crystallographic evolution of ice crystals as water exits the snow gun (see an example in Figure b).

These findings not only demonstrate the potential of feldspar additives to improve the efficiency and sustainability of artificial snowmaking, but also provide valuable insight into the crystallization pathways of supercooled water droplets in the presence of mineral ice-nucleating particles in natural and engineered environments.

Figure: (a) Images of the Snow Laboratory at La Molina. (b) Example snow density maps obtained with and without the use of feldspar additives.

[1] Kanji, Z. A., Ladino, L. A., Wex, H., Boose, Y., Burkert-Kohn, M., Cziczo, D. J., and Krämer, M.: Overview of Ice Nucleating Particles, Am. Meteorol. Soc., 58, 1.1-1.33, https://doi.org/10.1175/amsmonographs-d-16-0006.1, 2017.

[2] ]. Patent: “Artificial Snow Making Method And Product For Implementing The Method “ A. Verdaguer and M. Galvin https://uspto.report/patent/app/20190323753

[3] Daily, M. I., Whale, T. F., Kilbride, P., Lamb, S., John Morris, G., Picton, H. M., and Murray, B. J.: A highly active mineral-based ice nucleating agent supports in situ cell cryopreservation in a high throughput format, J. R. Soc. Interface, 20, 20220682, https://doi.org/10.1098/rsif.2022.0682, 2023

[4] Canet, J., Rodríguez, L., Renzer, G., Alfonso, P., Bonn, M., Meister, K., Garcia-Valles, M., Verdaguer, A.: Measurement report: Ice nucleation ability of perthite feldspar powder, EGU [preprint], https://doi.org/10.5194/egusphere-2025-5014, December 2025.

How to cite: Verdaguer, A., Canet, J., and Rodríguez, L.: Field Studies of Feldspar-Assisted Snowmaking: Effects on Snow Volume, Density, and Reflectivity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11937, https://doi.org/10.5194/egusphere-egu26-11937, 2026.

EGU26-12118 | ECS | PICO | CR5.1

Daily high-resolution SnowMicroPen Snow Stratigraphy measurements at a Swiss mountain site 

Leah Gaillard Festa, Bettina Richter, Lars Mewes, Benjamin Walter, and Matthias Jaggi

Snow density and specific surface area (SSA) are key parameters controlling snowpack stability, hydrological processes, and surface energy balance. Their accurate simulation is therefore essential for applications ranging from avalanche forecasting to climate modeling. However, these parameters are often time consuming to measure and are available at coarse vertical resolution. The SnowMicroPen (SMP) allows for high-resolution measurements of penetration force from which key microstructural parameters for instance snow density and SSA can be derived using parameterizations such as the one from  [Proksch et al., 2016] or [Calonne et al., 2020]. At the Weissfluhjoch research site located in the eastern Swiss Alps at 2536 m a.s.l, daily SMP measurements have been conducted by the SLF PhD students continuously since winter 2015–2016, resulting in a unique, long-term dataset documenting the seasonal evolution of alpine snowpack at high temporal (daily) and spatial (vertical) resolution.

Here, we present and analyze ten winters (2015–2025) of daily SMP measurements, combined with complementary manual observations, i.e. bi-weekly snow profile measurements, density cutter data, snow water equivalent (SWE) profiles, IceCube SSA measurements, and automated snow and meteorological observations. Post-processing steps, including the identification and correction of sensor offset effects, were applied to ensure comparability of the derived snow properties across the full multi-year dataset. This was crucial, as the data exhibited a clear offset that showed season-dependent behavior and strongly affected derived snow properties, particularly in low density snow ranges. SMP derived snow density and SSA were then evaluated against independent reference measurements across multiple winters.

Snow density showed good agreement with cutter and SWE-derived densities, with the strongest agreement observed for SWE from the full profile and calibration-period cutter data derived by [Calonne et al., 2020]. The SMP is limited to dry-snow conditions. Larger deviations were observed for fresh snow and under warm conditions. For SSA, SMP-derived values showed systematic deviations relative to IceCube measurements, particularly at higher temperatures.
This multi year, high temporal and vertical resolution dataset provides insight into the seasonal evolution of snow stratigraphy, densification, and microstructural changes in an alpine snow. The data allows for analyzing snow layer evolution across multiple winters, and how density and SSA respond to factors such as temperature gradients and densification processes. These findings highlight the potential of the SMP to improve understanding of snow microstructure which helps to improve representations of snow in climate and snowpack models.


References
Neige Calonne, Bettina Richter, H. L¨owe, C. Cetti, J. ter Schure, A. Van Herwijnen, C. Fierz, M. Jaggi, and M. Schneebeli. The rhossa campaign: multi-resolution monitoring of the seasonal evolution of the structure and mechanical stability of an alpine snowpack. The Cryosphere, 14(6):1829–1848, 2020. doi: 10.5194/tc-14-1829-2020.

M. Proksch, N. Rutter, C. Fierz, and M. Schneebeli. Intercomparison of snow density measurements: bias, precision, and vertical resolution. The Cryosphere, 10(1):371–384, 2016. doi: 10.5194/tc-10-371-2016.

How to cite: Gaillard Festa, L., Richter, B., Mewes, L., Walter, B., and Jaggi, M.: Daily high-resolution SnowMicroPen Snow Stratigraphy measurements at a Swiss mountain site, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12118, https://doi.org/10.5194/egusphere-egu26-12118, 2026.

EGU26-12232 | ECS | PICO | CR5.1

Development of a 2D high-resolution field method to measure liquid water content in snow 

Valentin Philippe, Michael Lombardo, Lars Mewes, and Benjamin Walter

The liquid water content (LWC) of snow is a key parameter controlling snowpack stability, runoff generation, and the timing of meltwater release (Vorkauf et al., 2021). With climate warming, rain-on-snow events and earlier snowmelt are becoming more frequent (Beniston et al., 2016), raising challenges for water management, hydropower production, flood warning, and avalanche forecasting. Despite its importance, accurate measurement of LWC in the field remains difficult. Existing methods, such as calorimetry, centrifugal separation, and dielectric sensors (Denoth et al., 1984), provide useful estimates but are limited by relatively high uncertainties (1-2% LWC) and low spatial resolution (> 3 cm). Hyperspectral imaging can resolve LWC variability at millimetre scale but is costly and impractical for routine fieldwork.

In recent years, the Snow Physics group at WSL/SLF has developed the SnowImager, a near-infrared (NIR) imaging instrument capable of capturing snow properties at high spatial resolution (Macfarlane et al., 2023). Using this instrument, we investigated the influence of liquid water on reflectance images by comparing the relative difference between a wet snow surface and its (re)frozen dry reference state. The obtained trend as a function of LWC is consistent with theoretical predictions based on a modified single scattering equation that accounts for both LWC and SSA. Building on this result, we developed a straightforward method to estimate LWC from reflectance images acquired with the SnowImager. Preliminary cold-lab and field tests confirmed the feasibility of this approach and demonstrated its potential to produce quantitative, high-resolution 2D maps of LWC.

We anticipate that the resulting 2D LWC field method will provide cryospheric researchers with a long-needed, practical, and precise tool to characterize the spatiotemporal dynamics of wet snow. This advancement will support improving wet snow avalanche forecasting, melt water runoff modelling, and climate impact assessments, while enhancing the SnowImager’s role as a versatile instrument for the international snow science community.

 

REFERENCES

Beniston, M., & Stoffel, M. (2016). Rain-on-snow events, floods and climate change in the Alps: Events may increase with warming up to 4 °C and decrease thereafter. Science of the Total Environment, 571, 228–236. https://doi.org/10.1016/j.scitotenv.2016.07.146

Denoth, A., Foglar, A., Weiland, P., Mätzler, C., Aebischer, H., Tiuri, M., & Sihvola, A. (1984). A comparative study of instruments for measuring the liquid water content of snow. Journal of Applied Physics, 56(7), 2154–2160. https://doi.org/10.1063/1.334215

Macfarlane, A. R., Dadic, R., Smith, M. M., Light, B., Nicolaus, M., Henna-Reetta, H., Webster, M., Linhardt, F., Hämmerle, S., & Schneebeli, M. (2023). Evolution of the microstructure and reflectance of the surface scattering layer on melting, level Arctic sea ice. Elementa: Science of the Anthropocene, 11(1), Article 00103. https://doi.org/10.1525/elementa.2022.00103

Vorkauf, M., Marty, C., Kahmen, A., et al. (2021). Past and future snowmelt trends in the Swiss Alps: The role of temperature and snowpack. Climatic Change, 165, Article 44. https://doi.org/10.1007/s10584-021-03027-x

How to cite: Philippe, V., Lombardo, M., Mewes, L., and Walter, B.: Development of a 2D high-resolution field method to measure liquid water content in snow, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12232, https://doi.org/10.5194/egusphere-egu26-12232, 2026.

EGU26-12655 | ECS | PICO | CR5.1

Identifying key physical processes in snow compaction at different strain rates 

Mathilde Bonnetier, Lars Blatny, Guillaume Chambon, Johan Gaume, and Maurine Montagnat

The mechanical behavior of snow is complex, as it depends on a variety of physical processes occurring at different scales, from the microstructure (sintering, bond breakage, etc.) to the scale of the snowpack and entire slopes. In particular, snow mechanical behavior is highly dependent on strain rate, with a ductile-to-brittle transition occurring at strain rates of about 10-4-10-3 s-1. It is important to develop comprehensive snow mechanical models accounting for this complexity for applications such as avalanche hazard evaluation, snowpack compaction or hydrological studies.

In this work, our objective is to build a continuous numerical model in a finite strain framework, that captures the key mechanical behavior of snow in a large range of strain rates. In particular, this model should be capable of properly retrieving the various deformation patterns observed in experiments, from quasi-homogeneous deformation in the ductile regime to the emergence of unstable localization patterns, such as compaction bands or cracks, typically observed in the brittle regime.

The model is based on an elasto-viscoplastic constitutive law, inspired by the Modified Cam Clay model, which is characterized by an elliptical yield surface. Two specific effects are included in the evolution of this yield surface throughout the deformation process: a hardening effect due to the compaction of the snow, and a viscous effect due to the competition between bond breakage and sintering of the microstructure. This law has been implemented in the software Matter [1] based on the Material Point Method (MPM). This method combines Lagrangian integration points and a fixed background mesh, which allows for computations of large deformations.

We performed 2D simulations of centimeter-scale samples (15mm x 15mm), undergoing uniaxial displacement-controlled compaction, at different strain rates between 1.8x10-6 and 7.5x10-3 s-1. These simulations are meant to reproduce the laboratory experiments of Bernard et al. [2], which were carried out in an X-ray microtomograph, providing reconstructions of the snow microstructure and deformation throughout the compression. Detailed comparisons between numerical and experimental results will be presented to evaluate the robustness of the numerical model.

In addition, a systematic sensitivity analysis was conducted to investigate the impact of the various physical processes considered in the constitutive law on the observed compaction patterns. Of particular interest is the role of sintering on the emergence and propagation speeds of localization bands. Finally, future adaptations of the model to investigate the propagation of instabilities in heterogeneous snowpacks will be discussed.

 

[1] Blatny, L. and Gaume, J.: Matter (v1): An open-source MPM solver for  granular matter, Geosci. Model Dev., 18, 9149–9166, https://doi.org/10.5194/gmd-18-9149-2025, 2025.

[2] Antoine Bernard. Etude multiéchelle de la transition ductile-fragile dans la neige. Science des matériaux [cond-mat.mtrl-sci]. Université Grenoble Alpes, 2023. Français. ⟨NNT : 2023GRALI027⟩. ⟨tel-04145610⟩

How to cite: Bonnetier, M., Blatny, L., Chambon, G., Gaume, J., and Montagnat, M.: Identifying key physical processes in snow compaction at different strain rates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12655, https://doi.org/10.5194/egusphere-egu26-12655, 2026.

EGU26-12973 | ECS | PICO | CR5.1

Modeling with SCHNAPS: the Snow Cover and High-resolutioN Atmospheric Processes System  

Dylan Reynolds, Samuele Viaro, Nander Wever, and Michael Lehning

Mass and energy exchanges between the cryosphere and the atmosphere affect the state of both systems, motivating the development of two-way coupled cryosphere-atmosphere models. For snow-atmosphere models, traditional atmospheric models are coupled to multilayer physics-based snow models and run in a large-eddy mode when simulating horizontal resolutions approaching 100m. For the CRYOWRF model in particular, the atmospheric model WRF was coupled to the snow model SNOWPACK. This approach has enabled detailed studies of snow-atmosphere feedbacks such as sublimation of drifting and blowing snow. However, the high computational cost of CRYOWRF limits its application to short spatio-temporal domains at scales relevant to drifting and blowing snow (<100m). This excludes research questions such as the role that blowing snow may play as an ice nucleation particle. A prior attempt to circumvent this experimental constraint by coupling the intermediate complexity atmospheric model HICAR and the snowpack model FSM2Trans yielded promising results but showed clear shortcomings when simulating drifting and blowing snow, as well as radiation-driven spatial melt patterns. This echoes work highlighting the importance of prognostic, physics-based models of surface albedo and blowing snow schemes which include vertical advection.

These considerations lead to the development of a two-way coupling between the physics-based SNOWPACK snow model and the intermediate-complexity atmospheric model HICAR. To capture mass exchange between the snow and atmosphere, blowing and drifting snow schemes similar to those in the CRYOWRF model are implemented. The resultant 2-way coupling of SNOWPACK to HICAR yields the Snow-Cover and High-resolutioN Atmospheric Processes System (SCHNAPS). Here we detail the coupling strategy, including a revised interface for SNOWPACK. Benchmarking runs at a 50m resolution are performed, showing the fractional increase in runtime attributed to using a snow model of higher physical complexity. A preliminary validation of SCHNAPS using distributed snow height measurements is presented. The improved representation of ice physics in SNOWPACK relative to NoahMP is also shown to improve the surface energy balance over a mountain glacier. Additionally, we present a comparison of blowing and drifting snow totals between SCHNAPS and CRYOWRF, as well as HICAR coupled to the intermediate complexity snow model FSM2Trans. SCHNAPS demonstrates how different representations of snowpack processes in a coupled snow-atmosphere model impacts snowpack evolution over the course of a season. This work sets the foundation for future studies of snow-atmosphere interactions in High Mountain Asia and the Antarctic via the SnowShifts Project.

How to cite: Reynolds, D., Viaro, S., Wever, N., and Lehning, M.: Modeling with SCHNAPS: the Snow Cover and High-resolutioN Atmospheric Processes System , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12973, https://doi.org/10.5194/egusphere-egu26-12973, 2026.

EGU26-13371 | ECS | PICO | CR5.1

Optical Determination of Snow Microstructure Parameters with the SnowImager instrument 

Adrian Zölly, Benjamin Walter, Lars-Hendrik Mewes, Martin Schneebeli, Henning Löwe, and Tobias Thomi

Extensive and reliable ground-truth measurements of snow properties play a crucial role in environmental science to validate models and remote-sensing products. Among the available methods, optics-based approaches offer a good compromise between measurement accuracy and sufficiently large coverage.

We present the technical details of the SnowImager as well as its data products. The SnowImager is a novel, rugged yet portable field instrument that uses near-infrared (NIR) imaging to determine physical snow properties. It enables fast, accurate, and standardized retrieval of two-dimensional specific surface area (SSA) images as well as vertically resolved density profiles, both with millimetre-scale resolution. The SnowImager can be used on vertical snow profiles as well as on the surface scattering layer of sea ice. It was jointly developed by the Swiss federal institute for snow- and avalanche research SLF and Davos Instruments AG.

Providing enhanced snow microstructure characterization, the SnowImager allows better understanding of the processes influenced by the physical properties of snow as well as of their spatial variability. Examples of such fields of use include snow physics, avalanche science and forecasting, meltwater runoff modelling and water storage management, energy balance analysis in climatic models and permafrost studies and albedo observations in systems including snow or a surface scattering layer on sea ice.

How to cite: Zölly, A., Walter, B., Mewes, L.-H., Schneebeli, M., Löwe, H., and Thomi, T.: Optical Determination of Snow Microstructure Parameters with the SnowImager instrument, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13371, https://doi.org/10.5194/egusphere-egu26-13371, 2026.

EGU26-15731 | PICO | CR5.1

Assessing the effects of uncertainty in windspeed and precipitation forcings on lateral snow redistribution in mountainous basins 

Rachel Corrigan, Adrienne Marshall, Christopher B. Marsh, and Andrew W. Wood

Snow-dominated montane watersheds provide critical ecological function, water storage, and water supply for downstream population centers across the globe. Recent literature suggests that hydrologic model uncertainty in these watersheds is largely driven by meteorological forcing uncertainty. Additionally, few models simulate lateral snow transport processes such as blowing snow and avalanche, meaning that the impact of forcing uncertainty on snowpack redistribution is unknown. This pair of limitations presents a distinct challenge for modelers in both identifying accurate model structures and identifying the drivers of simulated results. In this study, we ask how uncertainty in windspeed and precipitation forcing affects modeled lateral redistribution of snow in mountain basins. We hypothesize that windspeeds and precipitation from downscaled meteorological datasets require numerical correction for effective snow redistribution, and that the magnitude of these corrections will vary across geographic regions. Analyzing the impacts of these uncertainties allows us to determine how influential windspeed and precipitation forcings are on snow transport processes and on the spatial patterns of snow accumulation and melt dynamics.

We use the Canadian Hydrologic Model (CHM), to simulate snow accumulation and melt over five water years within a set of basins in the Sierra Nevada and Rocky Mountains in the United States that have extensive airborne lidar observations from the Airborne Snow Observatory (ASO). CHM runs over a triangular mesh with a six-layer snowpack energy balance model and lateral transport through blowing snow and avalanche. We use two climate forcing datasets with different underlying resolutions to evaluate the effects of windspeed and precipitation on modeled snowpack in mountainous terrain. ERA5-Land, a 9-km resolution dataset, is selected because its global coverage is advantageous for geographic generalizability. The CONUS404 product, a 4-km resolution dynamically downscaled dataset from ERA5 over the contiguous US, is selected to test a higher resolution product over the areas of interest. In each basin, windspeed and precipitation are perturbed to assess sensitivity and the resulting snowpack distribution.

We use observed SWE, snow cover, and derived snow disappearance date from SNOTEL, snow courses, and MODSCAG to evaluate model results using a standardized benchmarking process. This enables us to decipher whether corrections to windspeed and precipitation yield similar metrics despite different underlying redistribution processes. By evaluating models across two climatically distinct regions, we can assess whether numerical precipitation and windspeed adjustments improve snow simulations, and whether they are transferable or region-specific. We present an overview of the study and results demonstrating how uncertainty in meteorologic forcing propagates into lateral snow transport processes, which can provide guidance for improving snowpack simulations across complex mountainous terrain.

How to cite: Corrigan, R., Marshall, A., Marsh, C. B., and Wood, A. W.: Assessing the effects of uncertainty in windspeed and precipitation forcings on lateral snow redistribution in mountainous basins, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15731, https://doi.org/10.5194/egusphere-egu26-15731, 2026.

EGU26-16310 | ECS | PICO | CR5.1

 Long-term changes in snow cover dynamics across Germany (1950–present) 

Markus Drüke, Fabiana Castino, Grit Machui-Schwanitz, Bodo Wichura, Alice Künzel, Anett Fiedler, and Monika Rauthe

Snow cover is a highly sensitive indicator of climate change and plays a crucial role in hydrological processes, including groundwater recharge, runoff generation, and flood dynamics. Reliable long-term information on snow cover depth, extent, duration, and variability is therefore essential for climate monitoring, hydrological modeling, and impact assessments.

This study presents a comprehensive climatology of snow cover dynamics in Germany from 1950 to the present. The analysis is based on daily snow depth observations from the dense monitoring network of the Deutscher Wetterdienst (DWD) complemented by partner networks in Germany and neighbouring countries. All station data underwent rigorous quality control and homogeneity testing. The cleaned observational dataset was then interpolated onto a regular 1 × 1 km² grid using an optimal interpolation scheme that forms an important part of the operational DWD snow-melt forecast model SNOW4.

A suite of snow-related parameters was derived, including mean and maximum snow depth, snow cover duration, onset and disappearance dates, length of the main continuous winter snowpack, timing of peak snow depth, snow cover persistence, and winter snowpack stability.

The results reveal a widespread, statistically significant decline in almost all snow-related parameters across Germany over the last seven decades. The magnitude of the negative trends is strongly elevation-dependent: while lowlands and mid-elevation regions show pronounced reductions in snow cover duration and depth, high-altitude ridge and summit areas exhibit substantially weaker or – in the highest zones – partly insignificant trends.

This new high-resolution snow climatology provides a robust, consistent dataset for hydrological applications, climate change impact studies, water resource management, and the development of future climate services in the field of snow and water resources in Central Europe.

How to cite: Drüke, M., Castino, F., Machui-Schwanitz, G., Wichura, B., Künzel, A., Fiedler, A., and Rauthe, M.:  Long-term changes in snow cover dynamics across Germany (1950–present), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16310, https://doi.org/10.5194/egusphere-egu26-16310, 2026.

EGU26-16509 | ECS | PICO | CR5.1

Towards a Thermodynamically Consistent Phase-Field Model for Snow Metamorphism 

Henrik Jentgens, Thomas Kaempfer, and Mathis Plapp

The microstructure of snow undergoes continuous transformation in a process known as snow metamorphism. This evolving microstructure determines meso- and macroscopic optical, mechanical and thermal properties of the snowpack. Therefore, understanding the microstructural evolution on the pore scale is essential to forecast large-scale behavior.
By modeling phase transitions between ice and water vapor, we can treat fully coupled heat and mass transport on an arbitrary microstructure, allowing us to model dry snow metamorphism under temperature gradients and isothermal conditions alike. For this, a multi-phase-field model is used, by which we implicitly track the evolving microscopic ice-air interface. Compared to previous phase field models for dry snow metamorphism, a grand potential formulation is used to simplify the simulation of ice-vapor interfaces, as well as increasing the thermodynamic consistency. Thereby, we can treat various cross couplings between heat and mass transport like the Soret effect as well as surface diffusion and crystal growth dynamics. In this new model, near isothermal snow metamorphism is interpreted as sintering of ice grains. The thermodynamic properties of ice are modeled using CALPHAD data and humid air is modeled as a mixture of ideal gases.
We present our novel phase field model and validate it against semi-analytical solutions of the Stefan-problem and recently published experiments on simple geometries.

How to cite: Jentgens, H., Kaempfer, T., and Plapp, M.: Towards a Thermodynamically Consistent Phase-Field Model for Snow Metamorphism, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16509, https://doi.org/10.5194/egusphere-egu26-16509, 2026.

EGU26-17234 | PICO | CR5.1

A new cold ring wind tunnel facility for studying airborne snow metamorphism 

Benjamin Walter, Valentin Philippe, and Sonja Wahl

Recent studies suggests that drifting snow particles undergo snow metamorphism while being transported by wind, involving concurrent sublimation and vapor deposition, affecting particle size, shape, specific surface area, and isotopic composition [Walter et al., 2024; Wahl et al., 2024]. This newly identified process of airborne snow metamorphism (ASM) is particularly relevant in polar regions, where snow particles in saltation layers may be transported over long distances and durations before final deposition. As a result, this process strongly influences the microstructure of surface snow, with large scale implications for albedo and climate signals. Experimental investigations of ASM under laboratory conditions has so far been constrained by the lack of facilities providing well controlled boundary conditions.

Based on our experience with an exisiting but limitied ring wind tunnel (RWT), we developed a new wind tunnel in a cold laboratory designed to study airborne snow metamorphism under controlled flow and thermal conditions. The obround closed-circuit wind tunnel enables particle transport over long durations while maintaining stable boundary conditions. The facility is installed in a cold laboratory at the WSL Institute for Snow and Avalanche Research SLF, about 2m x 3m x 0.5m (W x L x H) in dimensions, and includes enhanced thermal control, a revised wind turbine integration reducing heating of the air, and snow surface temperature control, allowing independent regulation of air and surface temperatures.

We present a first comprehensive characterization of the flow field, including velocity distributions, spatial flow homogeneity, and turbulence properties across a range of wind speeds relevant for snow saltation and suspension. We further present a characterization of the thermal performance of the RWT, demonstrating improved temperature stability of the air and snow surface. The new ring wind tunnel provides a unique experimental facility for studying aerodynamic and thermodynamic impacts on snow particle evolution during snow transport. Generally, the new RWT facility additionally allows for studying a wide range of particle-flow and flow-surface (ice, snow, or water) interaction processes in turbulent cryospheric environments.

 

Walter B, Weigel H, Wahl S, Löwe H (2024) Wind tunnel experiments to quantify the effect of aeolian snow transport on the surface snow microstructure, The Cryosphere, 18, 3633-3652, https://doi.org/10.5194/tc-18-3633-2024

Wahl, S., Walter, B., Aemisegger, F., Bianchi, L., & Lehning, M. (2024). Identifying airborne snow metamorphism with stable water isotopes. Cryosphere, 18(9), 4493-4515. https://doi.org/10.5194/tc-18-4493-2024

 

How to cite: Walter, B., Philippe, V., and Wahl, S.: A new cold ring wind tunnel facility for studying airborne snow metamorphism, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17234, https://doi.org/10.5194/egusphere-egu26-17234, 2026.

EGU26-18027 | PICO | CR5.1

Multi-scale snowpack modeling in the Pyrenees using the Canadian Hydrological Model 

María Courard, Christopher Marsh, Isabelle Gouttevin, Hugo Merzisen, J. Ignacio López Moreno, César Deschamps-Berger, Eñaut Izaguirre, and Jesús Revuelto

In mountain ecosystems, snow is a critical resource that regulates hydrological processes, ecosystem dynamics, economical activities and downstream water availability. Accurately estimating snow at these highly heterogeneus environments remains a challenge, due to the strong spatial and temporal variability. The combination of snowdrift-permitting models and snowpack remote sensing observations can improve the accuracy of snowpack estimations across scales. The Canadian Hydrological Model (CHM) is a novel snow modeling framework that explicitly represents lateral snow transport processes over an irregular mesh. This study analyzes the impact of modelling spatial scales over three domains in the Pyrenees between 2019 and 2025 using CHM: the Izas Experimental Cathment (~10 km²), a portion of the Tena Valley (~100 km²), and a larger section of the mountain range (~1200 km²) using a snowdrift permitting model. Each domain is modelled using a different horizontal resolution, relative to the domain area, and driven by downscaled meteorological forcings. We analyze several snowpack properties, including snow covered area and snow depth, across the spatial scales, using point-scale snow survey stations, UAV-derived snow depth distribution maps at the catchment scale, Pléiades-derived snow depth maps at the valley scale and Sentinel 2 imagery at the mountain range scale. Error statistics, spatial efficiency metrics and scale breaks derived from semi variograms are used to evaluate the model performance. Preliminary results show that higher resolution simulations have a better representation of snow depth variograms and their scale breaks, and lower mean snow depth biases over the Izas catchment. However, snow depth is overestimated during the accumulation period and underestimated during the ablation season, and differences between the observed and simulated spatial snow distribution can be seen. This study improves our understanding of snowpack dynamics across spatial scales and of the horizontal resolution required for accurate snow simulations. Finally, this study enables the development of a remote sensing–based monitoring framework for the Pyrenees to improve snowpack simulation, which open new insights and allow more reliable forecasts.

How to cite: Courard, M., Marsh, C., Gouttevin, I., Merzisen, H., López Moreno, J. I., Deschamps-Berger, C., Izaguirre, E., and Revuelto, J.: Multi-scale snowpack modeling in the Pyrenees using the Canadian Hydrological Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18027, https://doi.org/10.5194/egusphere-egu26-18027, 2026.

EGU26-18196 | PICO | CR5.1

Interannual variability of the arctic snowpack: Results from long-term observations at Ny-Ålesund, Svalbard 

Hans-Werner Jacobi, Catherine Larose, and Jean-Pierre Dedieu

The Arctic is undergoing rapid environmental changes, with profound implications for snowpack dynamics, hydrology, and regional climate feedbacks. Ny-Ålesund, Svalbard (79°N), serves as an important site for documenting these changes due to its unique geographic location in the Arctic and its year-round research infrastructure. Here, we present the results of a comprehensive snowpack monitoring at Ny-Ålesund during five consecutive winter seasons (2018–2023).

Manual in-situ measurements of snow stratigraphy—including layer thickness, density, temperature, and hardness—were performed in weekly snow pits. While the region is traditionally considered as dominated by cold, shallow, and wind-affected "tundra” snow, recent winters exhibit increasing occurrences of snow characteristics not attributed to tundra snow, such as melt-freeze layers, internal ice accumulation, or wet snow. These anomalies are linked to rising temperatures, increased precipitation, and episodic winter rainfall events, which contrast sharply with the historical tundra snow regime. While the winter of 2019–2020 displayed classic tundra snow conditions, others winter seasons showed dominant maritime snow features. The statistical analysis of the observed physical snow parameters reveals a high variability of the snowpack characteristics. Such variability underscores the sensitivity of Arctic snowpack to local changes and highlights the challenges in predicting seasonal snowpack evolution. Simulating this enhanced variability will likely require snow models with enhanced capabilities.

This research emphasizes the importance of long-term, high-resolution observations in the remote Arctic. As the Arctic continues to warm, understanding these dynamics is essential for assessing broader environmental impacts, from permafrost degradation to shifts in regional water and biogeochemical cycles. The results call for sustained monitoring efforts and adaptive research strategies to address the evolving challenges posed by climate change in the Arctic.

How to cite: Jacobi, H.-W., Larose, C., and Dedieu, J.-P.: Interannual variability of the arctic snowpack: Results from long-term observations at Ny-Ålesund, Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18196, https://doi.org/10.5194/egusphere-egu26-18196, 2026.

EGU26-18218 | PICO | CR5.1

Spatial and Temporal Variabilities of Solar and Longwave Radiation Fluxes below a Coniferous Forest in the French Alps 

Jean-Emmanuel Sicart, Clare webster, Yves Lejeune, Richard Essery, and Nick Rutter

At high altitudes and latitudes, snow has a large influence on hydrological processes. Large fractions of these regions are covered by forests, which have a strong influence on snow accumulation and melting processes. Trees absorb a large part of the incoming shortwave radiation and this heat load is mostly dissipated as longwave radiation. Trees shelter the snow surface from wind, so sub-canopy snowmelt depends mainly on the radiative fluxes: vegetation attenuates the transmission of shortwave radiation but enhances longwave irradiance to the surface. 13 pyranometers and 11 pyrgeometers were deployed on the snow surface below a coniferous forest at the CEN-MeteoFrance Col de Porte station in the French Alps (1325m asl) during the winters 2016-17 and 2017-18 in order to investigate spatial and temporal variabilities of solar and infrared irradiances in different meteorological conditions. Sky view factors measured with hemispherical photographs at each radiometer location ranged from 1.5 to 3.5. In clear sky conditions, the attenuation of solar radiation by the canopy reached 96% and its spatial variability exceeded 100 W.m-2. Longwave irradiance varied by 30 W.m-2 from dense canopy to gap areas. In overcast conditions, the spatial variabilities of solar and infrared irradiances were reduced and remained closely related to the sky view factor. Comparing the measurements at different radiometer locations, we investigated the dependence of surface net radiation on the overlying canopy density. Of particular interest were the atmospheric conditions that favor an offset between shortwave energy attenuation and longwave irradiance enhancement by the canopy, such that net radiation does not decrease with increasing forest density (situations of “radiation paradox”). It was found that cloud effects on the shortwave transmissivity and longwave emissivity factors of the canopy have a strong impact on the subcanopy radiation fluxes: canopy largely counteracts the effects of clouds on the incoming radiation fluxes. As a result, variations in net surface radiation due to forest cover appear to depend largely on meteorological conditions: “radiative paradox” conditions were more frequent during the winter of 2017 than in 2018, which was cloudier and colder. As a result, variations in surface net surface radiation by canopy cover appear to be largely dependent on weather conditions: “radiative paradox” conditions were more prevalent during the winter of 2017 than in 2018, which was cloudier and colder.

How to cite: Sicart, J.-E., webster, C., Lejeune, Y., Essery, R., and Rutter, N.: Spatial and Temporal Variabilities of Solar and Longwave Radiation Fluxes below a Coniferous Forest in the French Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18218, https://doi.org/10.5194/egusphere-egu26-18218, 2026.

Snow is a major component of the hydrological cycle in cold environments. Snowpacks not only directly contribute to the local water cycle through snowmelt in late winter, but also constantly interact with local atmospheric water vapor through sublimation and vapor exchange throughout the winter. However, the widely used ‘traditional’ snow water isotope sampling method is destructive and temporally discrete, which limits the ability to capture the highly dynamic snow-liquid-vapor process within snowpacks. Therefore, at the Julinia site in Finland, we conducted the first winter field deployment of an innovative in-situ water isotope probe (WIP) system to sample cold and dry water vapor from snowpack layers and ambient air, where WIP was originally designed for use in trees and soils to study tree water uptake during the growing season. Water vapor sampled in-situ based on the direct vapor equilibrium method was continuously measured by a laser spectroscopy isotope analyzer (Picarro). Combined with ‘traditionally’ sampled water isotopes from event-based snowfall and snowpack layers, the temporal variation of δ18O and δ2H in different snowpack layers formed by different snowfall events illustrate the isotopic process of snowpack compaction, vapor exchange within the snowpack, and snowmelt. This approach provides an opportunity to better understand the long-overlooked isotopic difference between snowfall, snowpack, and snowmelt water, which can lead to non-negligible bias in partitioning ‘blue water’ and ‘green water’ in snow-dominated regions when using the stable water isotope techniques.

How to cite: Chen, Z., Marttila, H., and Ala-Aho, P.: In-situ high-resolution stable water isotope measurements of snowpacks in cold environments: opportunities for better understanding dynamic snowpack processes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18697, https://doi.org/10.5194/egusphere-egu26-18697, 2026.

EGU26-20575 | ECS | PICO | CR5.1

Climatic controls on global snow surface sublimation based on ERA5-Land 

Adrià Fontrodona-Bach, Harsh Beria, Denis Groshev, Thomas E Shaw, Catriona Fyffe, Isabella Anglin, Michael Lehning, and Francesca Pellicciotti

Sublimation of snow represents an often important but poorly constrained component of the hydrological cycle, especially at the global scale. Studies that estimate snow sublimation at point or catchment scales demonstrate a range of uncertainties in the contribution of sublimation to total winter snowfall, ranging from 5% to 90%. Although it is well established that dry, windy and clear-sky conditions favor snow sublimation, a modern, global-scale assessment of the climatic controls and regions where sublimation occurs and is relevant for snowpack evolution, glacier mass balance and water resources is lacking. Existing global efforts are limited by coarse resolution (~250 km) reanalysis data, leaving a critical gap in our understanding of sublimation’s contribution to the water balance across climates and regions. Here we present a global analysis of snow surface sublimation hotspots, using ERA5-Land reanalysis at 0.1° (~10 km) resolution from 1980 to the present. Comparisons with sublimation observations from eddy-covariance flux towers demonstrate that ERA5-Land underestimates sublimation rates, but performs favorably compared to estimates from other reanalysis (GLDAS, GLEAM, MERRA-2) products. Comparisons with station observations also demonstrate that ERA5-Land correctly reproduces global patterns of seasonal snow variability. 

Preliminary results show clear latitudinal, elevation and climatic controls on global surface sublimation. Hotspots of snow sublimation (>80 mm/year) are identified in the higher elevations of South America, North America and Asia, with contributions to total snow ablation ranging mostly from 10 to 20%. Hotspots of lower total annual surface sublimation (30 to 60 mm/year) lie in latitudes between 40 and 60 °N in dry climates, where the contributions to total snow ablation mostly range from 20% to 60%. The strongest surface sublimation hotspots in absolute and relative terms are identified in parts of Greenland and coastal Antarctica, where uncertainty is high as no sublimation observations from flux towers are available to compare with. We also investigate historical (1980-2025) changes in sublimation fluxes in response to warming and changing snow cover patterns. 

Our results highlight regions where surface sublimation may be a significant component of the hydrological cycle, with implications for water resources, glacier mass balance and snow–atmosphere interactions. Important uncertainties remain, particularly in complex mountain regions where the resolution of ERA5-Land data may not fully capture sublimation processes such as boundary layer warming and drying. Furthermore, drifting and blowing snow sublimation are not resolved in ERA5-Land. Future efforts should refine these global estimates by using higher-resolution simulations and improved representations of snow–atmosphere interactions to identify sublimation hotspots over complex terrain.

How to cite: Fontrodona-Bach, A., Beria, H., Groshev, D., Shaw, T. E., Fyffe, C., Anglin, I., Lehning, M., and Pellicciotti, F.: Climatic controls on global snow surface sublimation based on ERA5-Land, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20575, https://doi.org/10.5194/egusphere-egu26-20575, 2026.

EGU26-22324 | ECS | PICO | CR5.1

How snow, vegetation and soil properties influence soil temperatures in a permafrost environment (Trail Valley Creek, Western Canadian Arctic) 

Ephraim Erkens, Inge Gruenberg, Heidrun Matthes, Nick Rutter, and Julia Boike

Warming ground temperatures in the Arctic raise the need to forecast permafrost thaw. Seasonal snow cover is a crucial factor for ground temperatures as it can have a warming or cooling effect on the underlying soil, depending on snow cover timing and its physical properties. Vegetation and topography modulate snow distribution and affect the snow thermal insulation. However, the formation processes and resulting properties of Arctic snowpacks are difficult to represent in snow models and in-situ data is sparse. Further understanding of the interactions between snow, vegetation and permafrost and the deduction of empirical relationships could support the parametrization of snow in permafrost modeling.

We study how the ground thermal regime is influenced by the interplay of snow, vegetation, topography and climatic conditions. In particular, we evaluate the effect of snow density variation on the ground thermal regime. We present a novel dataset that combines air, surface and soil temperature, as well as soil moisture time series recorded from September 2024 to August 2025 with end-of-season snow depth distribution and high-resolution vertical snow density profiles. Temperatures and soil moisture were monitored using 60 TOMST TMS-4 loggers, distributed across different vegetation types and topographic features in the taiga-tundra ecotone (Trail Valley Creek, Northwest Territories, Canada). Snow density profiles were measured in March 2025 next to the TOMST loggers using a SnowMicroPen.

Our data shows several characteristic snowpack types which do not only differ in depth but also have a different layering structure. Low density snowpacks with high depth hoar fractions are most prominent in forested areas that are shielded from the wind, whereas leeward slopes can accumulate thick, high-density wind slab, regardless of vegetation. While snow depth is clearly one of the major drivers of soil temperature, the role of snow density is more complex.

Categorization of different tundra vegetation types with characteristic snow conditions and specific impact on permafrost vulnerability helps to refine permafrost models and constrain predictions of permafrost thaw.

How to cite: Erkens, E., Gruenberg, I., Matthes, H., Rutter, N., and Boike, J.: How snow, vegetation and soil properties influence soil temperatures in a permafrost environment (Trail Valley Creek, Western Canadian Arctic), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22324, https://doi.org/10.5194/egusphere-egu26-22324, 2026.

In an era characterized by urban densification and increasing pressures on urban space, along with the costs and availability of construction materials, the optimal design of infrastructure has become a critical focus. Furthermore, cold climate regions are experiencing the impacts of climate change, which manifest in altered precipitation patterns, resulting in more extreme storm events, including rain-on-snow events and increased freeze-thaw cycles. According to Maurin et al. (2024), rain-on-snow events have been identified as the leading cause of the highest observed runoff from green roofs, presenting significant challenges for urban areas in preventing flooding.

The present study aims to enhance understanding of the effects of climate variability and change on the hydrological performance of nature-based infrastructure, with a particular emphasis on green roofs during winter, especially in relation to snow and rain-on-snow events in cold climate regions. The goal is to develop guidelines that assist stakeholders in optimizing the design of nature-based solutions (NBS) infrastructure, ensuring they are resilient over time and effectively manage stormwater in a changing climate. This initiative addresses the current gap in research, particularly the lack of location-specific regulations that incorporate future climate projections for stormwater infrastructure design, giving decision-makers accurate information regarding the requirements for long-term and robust infrastructure design.

The study uses models of six different green and grey roof configurations developed in the SFI Klima 2050 project, calibrated for the winter season. These models utilize precipitation and temperature time series originated from high-resolution, convection-permitting climate models with hourly resolution and a 3x3 km gridded projection. Simulations for winter event separation (Melt, Rain and Rain-on-snow) are conducted following the methodology outlined in Maurin et al. (2024).

Results indicate that the changing climate will influence stormwater management strategies during winter, including higher runoffs of urban infrastructure due to rain-on-snow event with effects unevenly distributed across Norway (9 different cities studied). This pinpoints the need to combine the local future climate with hydrological models able to capture rain-on-snow events when planning and designing stormwater managements solutions that must remain effective under future climate scenarios. The findings have laid the groundwork for local guidelines aimed at ensuring climate-resilient design of nature-based infrastructure.

Maurin, N., Abdalla, E.H.M., Muthanna, T.M., Sivertsen, E., 2024. Understanding the hydrological performance of green and grey roofs during winter in cold climate regions. Science of The Total Environment 945, 174132. https://doi.org/10.1016/j.scitotenv.2024.174132

How to cite: Maurin, N., Abdalla, E. M. H., Landgren, O., and Sivertsen, E.: Assessing green roof hydrological performance during winter and rain-on-snow events under climate variability and change using high-resolution convection-permitting climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22740, https://doi.org/10.5194/egusphere-egu26-22740, 2026.

Current avalanche risk assessment relies heavily on manual snowpack observations and point-based meteorological data. Traditional forecasting requires personnel to physically enter high-risk terrain to perform stability tests and snow pit analyses, a process that is inherently dangerous, time-consuming, and limited by low spatial resolution. These manual "in-situ" measurements often fail to capture the complex stratigraphy and spatial variability of snow stability across entire slopes, leading to potential gaps in regional safety models.

To address these limitations, this research presents an integrated remote sensing framework utilizing Unmanned Aerial Systems (UAS) equipped with a multi-sensor payload. By synthesizing data from Ground Penetrating Radar (GPR), LiDAR, and multispectral cameras, we developed a non-invasive methodology for comprehensive snowpack characterization. The LiDAR sensors provide high-precision surface topography and snow depth measurements, while the GPR allows for the identification of internal stratigraphic boundaries and the estimation of snow density through electromagnetic wave propagation analysis. Concurrently, multispectral imaging assesses surface albedo and moisture content, offering insights into thermal degradation and surface hoar development.

The results of this integration are high-resolution 3D snow profile maps that allow for the quantitative assessment of snow hardness and density across broad, inaccessible slopes. By digitizing the snowpack structure at a granular level, this system provides forecasters with the data density required for accurate stability modeling without the necessity of human exposure to avalanche-prone zones. Ultimately, this UAS-based approach represents a paradigm shift in mountain safety, transitioning from discrete, high-risk manual sampling to continuous, remote, and data-driven hazard mitigation.

How to cite: Pistovčák, M.: High school students revolutionizing avalanche risk prediction using drones with mounted GPR, LiDAR and multispectral cameras, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2622, https://doi.org/10.5194/egusphere-egu26-2622, 2026.

EGU26-3022 | PICO | CR5.2

Artificial intelligence supported extended range Doppler radar: avalanche activity measurement and mitigation verification in Evolène, Switzerland 

Theo St Pierre Ostrander, Ólafur Stitelmann, Janine Wetter, Jonas Von Wartburg, Stéphane Vincent, and Maxence Carrel
The municipality of Evolène, located in the Swiss Alps, is exposed to significant avalanche hazard. Evolène comprises several settlements situated at the base of a mountain slope approximately 4.5 km in length with a topographic relief of 2000 m. During the winter of 1999, an intense storm cycle with significant snowfall accumulation rates triggered a destructive avalanche cycle with multiple fatalities and significant damage to property and supporting infrastructure. The slope affecting the municipality is characterized by numerous small and spatially distributed avalanche start zones, resulting in multiple avalanche paths that pose a significant and persistent threat to the valley’s population and infrastructure networks. As a result of the 1999 event, defense measures have been implemented to contribute to the overall mitigation scheme dealing with the avalanche hazard. These measures have been implemented over the past two decades, where a comprehensive avalanche protection and risk mitigation program has been deployed to reduce residual risk within the municipality. In the early 2000s, extensive structural measures, primarily snow-supporting/retaining measures in the start zones, were rapidly deployed. In a more recent project phase, the protection concept was expanded to include operational measures, notably remote avalanche control systems (RACS) and radar-based avalanche detection. In 2023, five RACS units and two radar systems were installed, with approximately twenty additional RACS units planned for phased installation in the coming years. The two radar systems are horizontally combined to provide continuous coverage of the entire slope, enabling the detection of avalanche events under all meteorological conditions at ranges exceeding 5.5 km. To enhance detection performance beyond conventional signal-processing algorithms, Geoprevent integrated a convolutional neural network–based artificial intelligence model, improving system sensitivity and reducing false detections. The system is actively used by local avalanche forecasters and practitioners for operational avalanche control and decision support, and delivered critical observational data during the active avalanche period of mid-April 2025. Although further improvements in detection accuracy remain possible, the generated data constitutes a valuable basis for evaluating system performance and for validating the spatial placement of current and planned RACS installations.

How to cite: St Pierre Ostrander, T., Stitelmann, Ó., Wetter, J., Von Wartburg, J., Vincent, S., and Carrel, M.: Artificial intelligence supported extended range Doppler radar: avalanche activity measurement and mitigation verification in Evolène, Switzerland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3022, https://doi.org/10.5194/egusphere-egu26-3022, 2026.

EGU26-6418 | ECS | PICO | CR5.2

Rapid mass movements triggered by rain-on-snow events associated with atmospheric rivers in West Greenland 

Andrea Securo, Renato R. Colucci, Charlotte Sigsgaard, Costanza Del Gobbo, Steffen R. Nielsen, Kristian Svennevig, and Michele Citterio

Rapid mass movements in cold mountain environments are an important geomorphic factor that shapes the landscape, as well as a potential source of geohazard. Although their triggering mechanisms have been investigated in multiple studies, the spatial and temporal distribution of these events is poorly known in most Arctic regions. Among rapid mass movements that can be triggered abruptly by precipitation and snowmelt, we report a large-scale event that involved Central West Greenland in July 2023. Rain-on-snow linked to an atmospheric river event triggered more than 150 slushflows in Disko Island (Qeqertarsuaq). Pre-post event remote sensing imagery was used to map the affected areas, while environmental monitoring data and climate reanalysis products provided insights into the atmospheric river event and its impact on a snow-dominated landscape. During the 18-hour event, cumulative precipitation peaked at 115 mm, with more than 80 mm in several areas among the most affected by debris and snowpack mobilization. We show how the extreme precipitation rates reached during this event are similar to those experienced during a few other rapid mass movement events (i.e., wet-slush avalanches, slush flows, and debris flows) documented in various locations across West Greenland. The implications of such extreme rain-on-snow events in the Arctic are still poorly known. We suggest increasing remote-sensing based efforts to monitor and map rapid mass movements in critical areas of the Arctic, as most of them go unnoticed when infrastructure or large-scale damage are not involved.

How to cite: Securo, A., Colucci, R. R., Sigsgaard, C., Del Gobbo, C., Nielsen, S. R., Svennevig, K., and Citterio, M.: Rapid mass movements triggered by rain-on-snow events associated with atmospheric rivers in West Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6418, https://doi.org/10.5194/egusphere-egu26-6418, 2026.

EGU26-8886 | ECS | PICO | CR5.2

From failure to fracture: concurrent field measurements of weak layer strength and fracture toughness. 

Melin Walet, Jakob Schöttner, Valentin Adam, Sirah Kraus, Florian Rheinschmidt, Philipp Rosendahl, Philipp Weissgraeber, Jürg Schweizer, and Alec van Herwijnen

Dry-snow slab avalanches are governed by two distinct but equally significant mechanical properties of weak snow layers: strength, which controls failure initiation, and fracture toughness, which governs whether an initial failure evolves into a self-sustaining crack. On inclined slopes, crack propagation occurs under mixed-mode loading, making avalanche release a combined multiaxial strength–fracture problem. A physically meaningful description of slab avalanche release requires both properties to be quantified together within the same weak layers.

In recent years, substantial progress has been made in characterizing these properties: multiaxial strength has been investigated extensively through laboratory experiments and numerical modeling, while mixed-mode fracture toughness has increasingly been measured directly in the field. However, these advances have largely remained disconnected. To date, strength and fracture toughness have not been measured simultaneously for the same weak snow layers, resulting in an incomplete mechanical description of the material's failure behavior.

Here, we therefore present recent experimental advances that enable direct field measurements of both failure and fracture properties of weak layers. We present a unique field-based dataset comprising multiaxial strength and mixed-mode fracture toughness measurements from two layers of buried surface hoar. Measuring both properties within the same layers allows us to construct both failure and fracture envelopes, providing a unified mechanical description of avalanche release. While both envelopes exhibit an elliptical shape, our results reveal contrasting behavior: weak layer strength is higher in compression than in shear, whereas fracture toughness is higher in shear than in compression. Relating these envelopes to weak layer microstructure, we qualitatively investigate how microstructural characteristics control failure initiation and crack propagation. Jointly constraining strength and fracture behavior with field data provides critical input for process-based avalanche release models and represents a significant step toward more physically consistent and reliable avalanche forecasting.

How to cite: Walet, M., Schöttner, J., Adam, V., Kraus, S., Rheinschmidt, F., Rosendahl, P., Weissgraeber, P., Schweizer, J., and van Herwijnen, A.: From failure to fracture: concurrent field measurements of weak layer strength and fracture toughness., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8886, https://doi.org/10.5194/egusphere-egu26-8886, 2026.

EGU26-10580 | ECS | PICO | CR5.2

Towards a model chain for an automated thalweg identification 

Paula Spannring, Christoph Hesselbach, Andreas Huber, and Jan-Thomas Fischer

To quantitatively assess properties of gravitational mass flows (GMFs), such as snow avalanches, we investigate the potential of an automated thalweg identification. In this context, a thalweg is defined as the main flow direction of a flow path in three-dimensional terrain. Along the main flow direction, two-dimensional representations, such as the relation of altitude to distance along the thalweg, provide a simplified representation of the three-dimensional GMF properties. Additionally, single quantitative characteristics describing the flow path can be identified from the thalweg. These thalweg analyses are used, for example, to compare different avalanche events or simulation outcomes and therefore to statistically analyze the underlying avalanche terrain. So far, automated thalweg identification has mainly been limited to individual flow paths on local scale.

The goal of the presented approach is to identify the two-dimensional thalweg representations of the GMFs from three-dimensional terrain on a regional scale automatically. For this, we extend an open-source model chain that delineates potential release areas (PRAs) based on three-dimensional terrain and computes their potential mobility and runout. In a further analysis, we can derive scalar characteristics along each thalweg, such as runout quantities. For example, these values can be used to analyze and validate the simulation of snow avalanches by comparing them to existing size classification approaches. 

The challenge is to identify the thalweg for every flow path automatically on a regional scale. For this purpose, PRAs are delineated from terrain-derived characteristics such as slope, surface roughness, wind exposure, and forest cover. Subsequently, PRAs are constrained by aspect criteria and subdivided into hydrologically meaningful subcatchments. For each PRA, we compute the runout using com4FlowPy, which is a computational module within the open-source avalanche simulation framework AvaFrame. It has been used to simulate several GMF processes (e.g., snow or rock avalanches) on a regional scale. With a well known, conceptual approach, it simulates the runout and intensity of GMFs. Within the runout simulation, the thalweg's location is computed as main flow direction for each release area by averaging the respective flow quantities. This model chain enables automatic thalweg delineation, requiring a digital elevation model and a suitable parametrization as model input. 

These thalwegs allow us to derive quantitative characteristics, such as runout length, corresponding angle and maximum flow velocity, for every flow path on a regional scale. These characteristics can be used for statistical analyses of the avalanche terrain.  When simulating snow avalanches of potential size, the applied parameterization can be validated by comparing these simulated thalweg characteristics with established avalanche size classification approaches. In addition, the analysis of simulated thalwegs enables comparisons of terrain characteristics between different study regions in terms of, for example, runout length, destructiveness, and the potential avalanche size. Identical input parameters are applied across the regions, ensuring that differences arise from terrain properties.

How to cite: Spannring, P., Hesselbach, C., Huber, A., and Fischer, J.-T.: Towards a model chain for an automated thalweg identification, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10580, https://doi.org/10.5194/egusphere-egu26-10580, 2026.

EGU26-12382 | ECS | PICO | CR5.2

Dynamical segmentation of avalanche debris from a time-series of Sentinel-1 SAR images 

Suvrat Kaushik, Guillaume James, Fatima Karbou, and Adrien Mauss

Mountain snow surfaces evolve through a combination of continuous processes, such as accumulation, melt, and redistribution, as well as abrupt, impulse-driven events, including snow avalanches. While C-band Synthetic Aperture Radar (SAR) time series have proven effective for avalanche mapping, most existing approaches rely on bi-temporal change detection or data-driven classification, treating avalanches as isolated events and neglecting the underlying temporal persistence and terrain-controlled spatial distribution of avalanche debris. In this study, we present a modified dynamical algorithm (m-DYN) for avalanche debris detection, which builds upon earlier applications of dynamical systems for mapping wet snow. The algorithm takes a SAR backscatter intensity ratio (BSR) image as an initial condition and iteratively evolves it toward a segmented image following a bistable dynamic.  This dynamics incorporates both a thresholding effect that tends to classify large BSR as avalanche debris and small BSR as background snow, and a physically consistent (topography-constrained) exchange of information between pixels at each iteration. Pixel coupling decreases with distance and is modulated by elevation differences, slope, and aspect, guiding the propagation of information along realistic avalanche flow paths and deposition zones. 

The methodology was evaluated over a study region of approximately 180 km2 in the vicinity of Davos, Switzerland, within the Swiss Alps, an area of high relevance for avalanche research. Two periods of pronounced avalanche activity were analysed: 20–24 January 2018 and 13–16 January 2019. During both intervals, high-resolution SPOT-6 imagery was acquired by the WSL Institute for Snow and Avalanche Research (SLF), and precise avalanche boundaries were mapped and are publicly available. These independently mapped avalanche outlines, together with associated ground-truth coverage information, serve as validation datasets. Sentinel-1 Level-1 Ground Range Detected (GRD) imagery at 20 m spatial resolution and a nominal 6-day revisit interval was used for the SAR time-series analysis.

Initial results demonstrate that the m-DYN algorithm generates spatially coherent and terrain-consistent avalanche debris maps, effectively suppressing noise and seasonal variability while preserving fragmented and low-contrast deposits. Compared to traditional threshold-based approaches, which produce patchy detections, the dynamical segmentation approach substantially improves the reconstruction of continuous avalanche flow paths while maintaining robust precision values. The method converges reliably within a limited number of iterations and shows strong agreement with independent validation datasets across both study periods, underscoring the potential of topography-aware dynamical algorithms for avalanche mapping using a SAR time series.

How to cite: Kaushik, S., James, G., Karbou, F., and Mauss, A.: Dynamical segmentation of avalanche debris from a time-series of Sentinel-1 SAR images, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12382, https://doi.org/10.5194/egusphere-egu26-12382, 2026.

EGU26-13917 | ECS | PICO | CR5.2

Self-supervised learning for automated avalanche detection from seismic and infrasound data 

Andri Simeon, Alec van Herwijnen, Johannes Aichele, Michele Volpi, Betty Sovilla, Pierre Huguenin, Johan Gaume, Andreas Fichtner, Pascal Edme, and Cristina Pérez-Guillén

Snow avalanches are among the deadliest natural hazards in mountainous regions. Yet avalanche activity is often still documented manually, and accurate avalanche release times are mostly missing. Automated monitoring systems equipped with seismic and infrasound sensors, combined with detection algorithms, could help record avalanche occurrences and provide accurate data on release time, size, and type. This comprehensive data on avalanche activity is indispensable for improving and validating avalanche forecasts and for implementing mitigation measures. At the Vallée de la Sionne (VDLS) test site in Switzerland, a combination of avalanche monitoring systems has been deployed for over two decades, including radars, cameras, seismic and infrasound stations. Additionally, avalanche researchers have manually documented and verified most avalanche events over the past 14 winter seasons to compile a unique avalanche catalogue.
To facilitate and automate avalanche detection, we aimed to implement two deep learning-based methods that scan continuous seismic and infrasound data separately in (near) real-time to detect and classify avalanche signals. Therefore, we leveraged the large volume of continuous data collected every winter at VDLS by adopting concepts from recent, powerful language models. Specifically, we pre-trained transformer networks in a self-supervised manner (i.e. without using expert labels) on a wide variety of signals mined from continuous seismic and infrasound data streams. The models receive fixed-length waveforms as input, partition them into sequential patches and compute patch-wise spectrograms. By training the models to reconstruct a portion of randomly masked patches, they learn to extract meaningful representations from the data, achieving silhouette scores of up to 0.6. This indicates good separability between avalanche and non-avalanche signals. Thus, these representations can later be used to automatically detect avalanches by fine-tuning a classifier on top. Moreover, combining predictions from the seismic and infrasound models has the potential to further improve (near) real-time avalanche detection.

How to cite: Simeon, A., van Herwijnen, A., Aichele, J., Volpi, M., Sovilla, B., Huguenin, P., Gaume, J., Fichtner, A., Edme, P., and Pérez-Guillén, C.: Self-supervised learning for automated avalanche detection from seismic and infrasound data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13917, https://doi.org/10.5194/egusphere-egu26-13917, 2026.

EGU26-17053 | ECS | PICO | CR5.2

Tracking avalanche nucleation in situ – A real-world experiment with embedded fibre optics 

Johannes Aichele, Pascal Edme, Simeon Andri, van Herwijnen Alec, Sovilla Betty, Huguenin Pierre, Gaume Johan, Fichtner Andreas, and Perez Cristina

Alpine mass movements pose a considerable risk to people and infrastructure. Snow avalanches pose a particularly prominent risk due to their widespread occurrence and potential catastrophic consequences. While significant advances have been made over the last decades to forecast avalanches, the spatio-temporal conditions that lead to avalanche release remain elusive. In fact, the problem of avalanche release is comparable to earthquake nucleation: An earthquake rupture and the fracture of a snow slab avalanche share the same underlying physics. As in the case of earthquakes, the observation of the rupture process of avalanches is limited to sensors in the farfield, such as seismic and infrasound arrays, and optical and radar methods, as well as laboratory experiments. While laboratory observations, far-field measurements on experimental test sites, and numerical simulations allow us to paint an ever more precise picture of the physics of avalanche nucleation, in situ measurements of crack propagation in the near-field of a real-world avalanche remain inaccessible so far.

How to perform such a measurement, which would not only allow us to understand the underlying physics better, but also might open new pathways to measuring precursory processes?

We designed a field experiment tackling the in situ observation of crack propagation and precursory processes. Leveraging a dense grid of seismic sensors we aim to capture the deformation in the nearfield prior, during, and after avalanche nucleation with Distributed Acoustic Sensing (DAS). In total, more than 3 km of fibreoptic cable were pulled from the top into the the steep slopes of Brämabuel near Davos (Switzerland) in autumn 2025. The cables were installed prior and during the first significant snowfall of the season, on known avalanche release slopes. Hence, they are placed centimeters below the expected weak layers, thus effectively making them an embedded strain sensor in a real-world experiment. To increase the probability of capturing the nucleation process, our DAS interrogator continuously samples at 2 m and 200 Hz, with the possibility to increase sampling rates to 1000 Hz for periods of increased avalanche risk. This continuous high spatio-temporal sampling will allow us to differentiate naturally and human-triggered slabs; in fact, skiers are easily identified in the data. In this talk, we will report on the first measurements of the 2025/2026 season and highlight the monitoring potential of our installation;

How to cite: Aichele, J., Edme, P., Andri, S., Alec, V. H., Betty, S., Pierre, H., Johan, G., Andreas, F., and Cristina, P.: Tracking avalanche nucleation in situ – A real-world experiment with embedded fibre optics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17053, https://doi.org/10.5194/egusphere-egu26-17053, 2026.

EGU26-17206 | ECS | PICO | CR5.2

Climate-driven changes in avalanche activity in the Haute-Maurienne valley (French Alps) over the period 1950–2100 based on machine-learning modelling 

François Doussot, Léo Viallon-galinier, Nicolas Eckert, and Pascal Hagenmuller

Snow avalanches in alpine environments are influenced by climate change. Assessing their long-term evolution remains difficult due to the scarcity of temporally consistent observation records. This lack of homogeneous data complicates the attribution of past changes to climate drivers and the development of credible future projections based on climate scenarios. To address these limitations, we develop a machine learning model that links avalanche observations with simulated meteorological and snowpack properties at a daily scale. A gradient-boosting regression model is trained to estimate daily avalanche counts, using weather and snow conditions derived from simulations. The analysis is conducted for a well-instrumented alpine catchment, the upper Haute-Maurienne valley in the French Alps, where approximately one hundred avalanche paths are monitored on a daily basis. We focus on avalanche events that reach predefined observation thresholds located at elevations of around 1800 m a.s.l. We show that particular attention to data quality and consistency has to be paid: accounting for uncertainties in avalanche release dates and restricting the training phase to a recent period with homogeneous observations are key prerequisites to obtain consistent results. Once trained, the model is first applied to reconstruct avalanche activity over the period 1958–2023 using reanalysed snow and meteorological data. It is then used to compute the evolutions of the avalanche activity between 1950 and 2100 using a downscaled ensemble of snow–climate simulations. Changes in avalanche activity are assessed using three complementary indicators corresponding to annual, monthly and weekly time scales. The reconstructed historical time-series indicates a marked decline in avalanche activity, with an average reduction of about 9 % per decade in the annual number of avalanches since 1958, mainly due to a decrease in the spring avalanche activity, while extreme avalanche cycles exhibit a more moderate decline. Future projections suggest a continued downward trend. Under the RCP4.5 and RCP8.5 scenarios, annual avalanche counts are projected to decrease by roughly 5 % and 9 % per decade, respectively, again largely driven by changes in spring conditions. Extreme avalanche activity is also expected to weaken, although at slower rates, with projected decreases in the 30-year return level of about 2 % per decade for RCP4.5 and 5 % per decade for RCP8.5. These climatic trends are associated with climate-induced changes in snowpack and meteorological variables through the use of machine-learning interpretation approaches. Overall, this study provides a quantitative assessment of climate-driven changes in avalanche activity for a representative alpine valley, combining machine-learning approaches with physically based snow-climate simulations.

How to cite: Doussot, F., Viallon-galinier, L., Eckert, N., and Hagenmuller, P.: Climate-driven changes in avalanche activity in the Haute-Maurienne valley (French Alps) over the period 1950–2100 based on machine-learning modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17206, https://doi.org/10.5194/egusphere-egu26-17206, 2026.

EGU26-18300 | ECS | PICO | CR5.2

Rain on snow (ROS) events in the Italian Alps 

Carlo Bee and Mauro Valt

In the Alps, numerous studies indicate that winter precipitation, measured in millimetres of water equivalent, does not exhibit any specific temporal trend. However, in recent years, the altitude of reliable snow cover has increased, whereas the snow depth on the ground, the amount of fresh snow, and the snow water equivalent (SWE) have decreased.

An investigation of the databases of Italian avalanche services affiliated with the Interregional Association for coordination and documentation of snow and avalanche problems (AINEVA), revealed an increase in rain on snow (ROS) events at all altitudes, even the highest above 2200 m. The analysis of data collected throughout the Italian Alps over a 20-year period (2006-2025) confirmed that spontaneous avalanche activity is greater on days with ROS.

Analysis conducted in the Dolomites, a range of the eastern Italian Alps, at six stations at different altitudes, further confirmed the increase in rainy days, especially in February and at medium and low altitudes. In the study area, the number of days with precipitation in the period 2016-2025 decreased by 25% compared to the previous decade, indicating more intense episodes, as total precipitation does not show significant variations. The number of snowy days decreased by 33%, further indicating a change in the snow-to-rain regime. Over the last 30 years, the snowfall limit increased by as much as 240 m in January and over 420 m in February.

How to cite: Bee, C. and Valt, M.: Rain on snow (ROS) events in the Italian Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18300, https://doi.org/10.5194/egusphere-egu26-18300, 2026.

EGU26-20362 | ECS | PICO | CR5.2

Glide-snow avalanche initiation: The influence of liquid water on snow-surface friction 

Rosa Schnebli, Miguel Cabrera, Alec Van Herwijnen, Johan Gaume, and Grégoire Bobillier

Glide-snow avalanches occur when the entire snowpack slowly slides along the ground. Although liquid water at the snow–soil interface is known to play a role in glide-snowavalanche initiation, the mechanical behaviour at this interface remains poorly understood (Ancey & Bain, 2015) (Fees et al., 2024). These full-depth avalanches pose a significant risk to alpine infrastructure, as they are difficult to forecast and often involve large volumes.

This study investigates the influence of liquid water content, normal stress, and surface roughness on the shear strength of the snow–soil interface using controlled cold- laboratory experiments. Artificially produced snow is compacted and cut into cylindrical samples with a diameter of 8 cm, which are then sheared on two non-porous surfaces: a geotextile and a slate. Liquid water content at the interface is systematically increased through controlled heating of the basal surface, while shear force and displacement during the experiment are continuously measured, and interfacial liquid water content is quantified immediately after each test.

The experiments exhibited strain-softening behaviour under all conditions. Under dry conditions, peak shear strength increased with both idle time (the duration of surface contact before shearing) and applied normal load, while the Mohr–Coulomb friction angle remained constant for each surface. Increasing idle time resulted in a parallel upward shift of the yield surface toward higher shear strengths. Under wet conditions, the peak shear strength remains roughly stable with increasing interfacial liquid water content; shear behaviour was primarily governed by surface type and normal load.

Our findings indicate that, in addition to liquid water content, interface mechanics and surface properties play an important role in glide-snow avalanche release. The results provide new experimental insight into basal friction processes and contribute to an improved conceptual understanding of glide-snow avalanche initiation.

References

Ancey, C., & Bain, V. (2015). Dynamics of glide avalanches and snow gliding. Reviews of Geophysics.

Fees, A., Lombardo, M., van Herwijnen, A., & Schweizer, J. (2024). Glide-snow avalanches: insights from spatio-temporal soil and snow monitoring.

How to cite: Schnebli, R., Cabrera, M., Van Herwijnen, A., Gaume, J., and Bobillier, G.: Glide-snow avalanche initiation: The influence of liquid water on snow-surface friction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20362, https://doi.org/10.5194/egusphere-egu26-20362, 2026.

EGU26-21871 | ECS | PICO | CR5.2

Drivers of Flow Channel Formation on Snow Surfaces: Rain versus Melt-Water – A Case Study in the Austrian Alps 

Veronika Hatvan, Andreas Gobiet, and Ingrid Reiweger

Flow channels on the snow surface are a common phenomenon frequently observed and reported to avalanche warning services. An accurate interpretation of field observations and an understanding of the underlying physical processes are crucial for the assessment of snowpack stability. Flow channel formation is typically associated with rain-on-snow (ROS) events and is often interpreted as an indicator of the approximate elevation of the snow line, a key factor in forecasting wet-snow avalanche activity and the formation of crusts and crust-related weak layers. However, recent observations of flow channel development, without significant liquid precipitation, challenge the assumption that ROS events are the sole cause of their formation.

In this study, we quantitatively compare liquid water input into the snowpack from melt processes to the amount of rain during a documented flow channel formation event. Using a combination of field observations, energy balance calculations and model simulations, we demonstrate that, at least in our case study, meltwater was the predominant driver of flow channel formation. Our results indicate that more than 97% of the total liquid water input originated from melt, while rain contributed only roughly 2%. These findings highlight the need for a revised interpretation of flow channel formation, suggesting that meltwater-driven flow channels may be more significant than previously assumed.

How to cite: Hatvan, V., Gobiet, A., and Reiweger, I.: Drivers of Flow Channel Formation on Snow Surfaces: Rain versus Melt-Water – A Case Study in the Austrian Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21871, https://doi.org/10.5194/egusphere-egu26-21871, 2026.

EGU26-22447 | ECS | PICO | CR5.2

Crack arrest in dry snow slab avalanches: Assessing the feasibility of man-made structures to stop crack propagation 

Francis Meloche, Ron Simenhois, Don Sharaf, Ethan Greene, and Johan Gaume
Large dry snow slab avalanches are responsible for most fatalities in Europe and also affect infrastructure such as roads, railways, ski resorts, and villages worldwide. Several decades of research focusing on crack propagation in weak snow layers have uncovered multiple mechanical processes leading to larger avalanches. A key finding is the transition from anticrack propagation (collapse of the weak layer) to a very fast shear-based propagation regime, in which crack speed can approach the longitudinal wave speed of the slab and is most likely associated with larger avalanches. However, there is still a lack of understanding regarding crack arrest mechanisms and the final propagation extent. Recent studies suggest that crack arrest processes can differ depending on scale related to both propagation regime, as well as crack arrest may or may not involve slab fracture.
This work focuses on large-scale crack arrest in the shear-based propagation regime, involving slab fractures in the cross-slope direction. The practical objective of this study was to test the feasibility of a ridge-like structure oriented in the downslope direction that could potentially promote slab fractures, stop crack propagation, and limit avalanche size during avalanche control operations. We used a numerical method called the Depth-Averaged Material-Point Method (DAMPM), which can reproduce all mechanical processes relevant to large avalanche release. Using this method, we simulated three different slope configurations to study cross-slope propagation in the presence of the ridge-like structure: (1) a simple planar slope 10 m long and 30 m wide, (2) an analytical bowl-shaped slope 120 m long and 80 m wide, and (3) a real, complex 3D terrain of the Stanley Path in Colorado.
For each slope configuration, we added a ridge-like feature where slab thickness—and correspondingly slab strength—was reduced, promoting slab fractures at the structure. Our results show that the structure dimensions are less important than the minimum slab depth covering the structure in discriminating between crack arrest and propagation through the structure. However, near the threshold slab depth value separating arrest from propagation, the structure dimensions—specifically the structure dimension ratio (height over width)—can influence whether arrest or propagation occurs. These results were consistent across all three slope configurations. Finally, simulations on the real 3D complex terrain of Stanley Path show realistic slab fracture behavior over complex topography, including both tensile and compressive fractures. These results contribute to an improved understanding of crack arrest mechanisms involving slab fracture.

How to cite: Meloche, F., Simenhois, R., Sharaf, D., Greene, E., and Gaume, J.: Crack arrest in dry snow slab avalanches: Assessing the feasibility of man-made structures to stop crack propagation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22447, https://doi.org/10.5194/egusphere-egu26-22447, 2026.

EGU26-22941 | PICO | CR5.2

Avalanche Laboratory Nordkette/Innsbruck – On the technical design of the Arzler Alm avalanche test site 

Engelbert Gleirscher, Anselm Köhler, Matthias Granig, Christian Tollinger, Jannis Aust, Christian Demmler, Gebhard Walter, and Jan-Thomas Fischer

The south-facing Arzler Alm avalanche path above Innsbruck, Tyrol, has a release area at approximately 2300 m a.s.l. on the Nordkette range and a runout zone reaching the immediate vicinity of an Innsbruck city district at about 650 m a.s.l. Following several very large avalanche events during the last century, extensive mitigation measures were constructed, including multiple breaking mounds and a catching dam, designed to withstand avalanche volumes of up to 1 million cubic meters. An exceptional snowstorm during the winter of 2018/19 triggered a large avalanche that caused substantial forest damage and highlighted the continued necessity of these protection structures.

During recent renovation works, a comprehensive measurement system was installed in the uppermost breaking mound. This structure is 5 m high, wedge-shaped, and approximately 10 m wide. Force measurements on a structure of this scale provide a rare opportunity to improve current engineering standards by describing avalanche-obstacle interactions. The measurement system consists of multiple 0.25 m² pressure plates installed on the mountain-facing sides of the breaking mound and record data at 10 kHz. These sensors capture both frontal impact forces and shear forces generated during flow deflection along the lateral flanks. To place local force measurements into the context of entire avalanche events and to quantify avalanche occurrence frequency, a state-of-the-art avalanche radar observes the full avalanche track continuously. The setup is complemented by video cameras from multiple viewing angles and allows future expansion with additional instrumentation, such as seismic sensors, fiber-optic sensing systems, and optical velocity measurements.

The test site has been operational since early 2026. We primarily present the technical design, site layout, and instrumentation and in case discuss data collected from avalanches during the current winter season. However, as the experiments rely entirely on natural avalanche activity and the statistical recurrence interval for avalanches reaching the mitigation structures is approximately one event per season, the availability of force measurements cannot be guaranteed for every year.

The Arzler Alm Avalanche Test Site is part of the Avalanche Laboratory Nordkette (Innsbruck, Austria), where recording of forces in snow fences, observations of glide snow activity and measurements with in-flow sensors in artificially released avalanches are performed. It complements other existing full-scale European avalanche research facilities such as Vallée de la Sionne (Valais, Switzerland) and Ryggfonn (western Norway). The year-round accessibility enables detailed manual field campaigns, including investigations of avalanche deposits, snow compaction in front of breaking mounds, and volumetric and entrainment processes. The south facing, large altitude range combined with significant new snow amounts during northwesterly snowstorms promotes avalanches that may transition from cold, dry flow regimes at release to warm, wet conditions in the deposition zone, making this new site particularly valuable for the large variety of avalanche release types, flow regimes and their evolution.

How to cite: Gleirscher, E., Köhler, A., Granig, M., Tollinger, C., Aust, J., Demmler, C., Walter, G., and Fischer, J.-T.: Avalanche Laboratory Nordkette/Innsbruck – On the technical design of the Arzler Alm avalanche test site, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22941, https://doi.org/10.5194/egusphere-egu26-22941, 2026.

EGU26-2074 | ECS | Posters on site | HS2.1.4

Temporal variability of catchment storage-discharge characteristics and their driving mechanisms in cold region 

Zhicheng Xu, Yinjun Zhou, and Lei Cheng

The catchment storage-discharge characteristics (CSDC) are usually the highly sensitive parameters in hydrology model and fundamentally decide the baseflow simulation performance. With dramatic climate change, several recent studies had found significant trend of the power-law parameter of CSDC (b0) in cold region. However, studies about the temporal variability of b0 and its driving mechanism in cold region are less consistence because of differences in study area and time scale. In this study, the b0 was firstly calculated from daily recession event in 315 cold catchments, after which the time-varying rule of b0 and its driving mechanism was investigated at events, warm period and decades scales. The results show that the set of calculated b0 have a median of 2.1 around all study catchments and are great different between flow recession events in a specific catchment with the median of its variance in all study catchments is equal to 2.3. Moreover, the b0 increased within warm period in most (78%) cold catchments and had also an increase on the decades scale in 63% cold catchments, stating a significant time-varying characteristic. Correlation analysis presents that permafrost extent degradation, increases in both precipitation (P) and terrestrial water storage (TWS) play the positive roles in b0, while increasing PET play the negative role on the contrary. On the events scale, potential evaporation (PET) is the main control of the b0, followed by the permafrost extent, while P and TWS take a slightly positive effect. During the warm period, permafrost thawing overtakes PET as the main control of the b0, followed by the PET, and the effect of P and TWS can be not negligible. On the decade scale, climate change (i.e, climate warming and wetting) caused permafrost degradation and increases in both P and TWS, which has further increased the b0. These results are of great significance for improving the understanding of the catchment storage-discharge process, and highlight that traditional hydrology modelling with constant CSDC could result in systematic bias in baseflow simulation and prediction in cold region.

How to cite: Xu, Z., Zhou, Y., and Cheng, L.: Temporal variability of catchment storage-discharge characteristics and their driving mechanisms in cold region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2074, https://doi.org/10.5194/egusphere-egu26-2074, 2026.

EGU26-2612 | ECS | Posters on site | HS2.1.4

Evaluating a Long Short-Term Memory (LSTM) approach for Snow Water Equivalent (SWE) downscaling and hydrological modeling in mountainous terrain 

seyedeh hadis moghadam, Richard Arsenault, André St-Hilaire, and Frédéric Talbot

In the context of the global hydrological cycle, runoff generated from snowmelt plays a key role in water availability, particularly in cold and mountainous regions. In many parts of Canada and the western United States, mountain snowpacks act as natural reservoirs by storing precipitation during cold seasons and releasing it during spring and summer. Accurate estimation of snow water equivalent (SWE) is therefore essential for hydropower reservoir operation, snow-related hazard assessment, and hydrological modeling. However, the coarse spatial resolution of widely available SWE products in northern latitudes, combined with complex mountain topography, introduces substantial uncertainty in their direct application to hydrological models. High-resolution SWE mapping remains a major challenge in these environments. In this study, we propose a multifactor SWE downscaling framework based on a Long Short-Term Memory (LSTM) deep learning approach, applied to the Nechako River watershed in British Columbia, Canada. The framework uses ERA5-Land SWE at 10 km resolution as the target variable, with predictor variables including precipitation, minimum and maximum temperature, solar radiation, and 2-m dewpoint temperature, together with static physiographic information such as elevation and land cover. Daily data from 1981 to 2024 are considered. The model is trained and evaluated at the 10 km resolution before being applied to generate SWE at 5 km resolution, corresponding to the spatial resolution of the CEQUEAU hydrological model. The downscaled SWE fields are designed to retain the large-scale snow patterns provided by ERA5-Land, while adding more spatial detail based on local elevation and land cover. Current work focuses on incorporating these downscaled SWE estimates into the CEQUEAU hydrological model and comparing the resulting runoff simulations with those obtained using CEQUEAU’s internal SWE representation. Rather than aiming to demonstrate clear improvements at this stage, the goal is to better understand how different SWE inputs influence the simulated hydrological response. Preliminary results suggest that LSTM-based downscaling offers a flexible and promising way to generate intermediate-resolution SWE fields in mountainous regions. This approach shows potential as a practical link between coarse-resolution reanalysis products and distributed hydrological models used for water resources and hydropower studies.

How to cite: moghadam, S. H., Arsenault, R., St-Hilaire, A., and Talbot, F.: Evaluating a Long Short-Term Memory (LSTM) approach for Snow Water Equivalent (SWE) downscaling and hydrological modeling in mountainous terrain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2612, https://doi.org/10.5194/egusphere-egu26-2612, 2026.

EGU26-3886 | ECS | Orals | HS2.1.4

Reimagining how Andean glaciers buffered past streamflow droughts  

Rodrigo Aguayo, Harry Zekollari, Jordi Bolibar, Marit van Tiel, Álvaro Ayala, Lander Van Tricht, and Lizz Ultee

Climate change intensifies water scarcity by increasing the frequency of streamflow droughts. Glaciers play a key role in moderating these events by regulating runoff, but their ongoing retreat threatens this natural resilience. Despite case-specific advances, the regional role of Andean glaciers in shaping streamflow droughts across complex climates and landscapes remains highly uncertain. To address this gap, we use a hybrid glacio-hydrological model that combines process-based glacier mass-balance and ice-flow dynamics with a data-driven runoff representation, allowing us to capture both long-term glacier evolution and short-term hydrological responses. This model is applied to a newly developed dataset of 257 glacierized catchments spanning the Andes (“AndeanGC”; 5–56ºS), which consolidates harmonized hydrological observations, remotely sensed glacier characteristics, and gridded meteorological forcing. The hypothetical future glacier extents correspond to projections under three warming storylines that represent plausible global outcomes: a Paris-aligned pathway limiting warming to 1.5 °C, a current-policy trajectory leading to approximately 2.8 °C of warming, and a high-emission pathway reaching about 4.0 °C. We find that glaciers historically provided substantial buffering of streamflow droughts, but this effect diminishes as glaciers shrink. If past droughts had occurred under the smaller glacier extents projected for the late 21st century under current climate policies, their severity and spatial extent would have increased substantially. Consequently, regional water stress would have intensified markedly. These hypothetical scenarios reveal the previously unquantified regional influence of glaciers on past droughts and illustrate the broader consequences of their decline for water resources. They also highlight the critical need to communicate these changes effectively to support climate-resilient planning and policy.

How to cite: Aguayo, R., Zekollari, H., Bolibar, J., van Tiel, M., Ayala, Á., Van Tricht, L., and Ultee, L.: Reimagining how Andean glaciers buffered past streamflow droughts , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3886, https://doi.org/10.5194/egusphere-egu26-3886, 2026.

EGU26-4540 | ECS | Posters on site | HS2.1.4

Snowmelt–Baseflow Lags as Indicators of Elevation-Dependent Storage Buffering in Snow-Dominated Mountain Catchments 

Johnmark Nyame Acheampong and Michal Jenicek

Snowmelt is a critical seasonal water source in mountain catchments, yet the dynamics of catchment water storage and release, as well as the redistribution of snowmelt signals into low-flow periods, remain poorly constrained, particularly across the snow–rain transition. In this study, we focus on one diagnostic question: how long does the snow signal persist before it emerging in baseflow, and how does that lag change with elevation and snow regime? We analyse 88 near-natural mountain catchments in Czechia and Switzerland using HBV-Light simulations of snow water equivalent (SWE) and baseflow and apply wavelet coherence to quantify phase-derived SWE–baseflow lags as a signal-based indicator of storage modulation. Across both regions, SWE and baseflow exhibit stable annual coupling, with SWE consistently leading baseflow. Mean lags are systematically longer in higher, colder, and snow-richer catchments, consistent with stronger storage buffering and delayed meltwater release. At the regional scale, the characteristic lag is ~69 days in Czech catchments and ~100 days in Swiss catchments, and the lag increases with elevation in both countries. These storage-linked delays align with stronger snow support to summer baseflow at higher elevations, while mid-elevation catchments near the snow–rain transition show shorter lags and weaker persistence of snow influence. This lag-based indicator provides a compact, transferable way to diagnose where snowmelt most strongly sustains baseflow through storage buffering, and where this mechanism is most likely to weaken as snow seasons shorten under warming.

How to cite: Acheampong, J. N. and Jenicek, M.: Snowmelt–Baseflow Lags as Indicators of Elevation-Dependent Storage Buffering in Snow-Dominated Mountain Catchments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4540, https://doi.org/10.5194/egusphere-egu26-4540, 2026.

EGU26-6027 | ECS | Posters on site | HS2.1.4

Evaluation of the performance of a database for snow water equivalent in southern Quebec, obtained using a spatialised particle filter 

Ralph Bathelemy, Marie-Amélie Boucher, Sergio Andrés Redondo Tilano, and Justine Hamelin

Université de Sherbrooke (UdeS) produced a snow water equivalent (SWE) database for southern Quebec, Canada, using a spatialised particle filter, the snow module of the distributed hydrological model Hydrotel, and two types of snow observations (manual snow surveys, and automated sonic sensors). This gridded database has a spatial resolution of 10 km and covers the southern part of the province of Quebec, below 53°N. This database is used operationally as part of the government’s official flood forecasting system but has never been compared to other similar gridded datasets. This work therefore aims to compare the UdeS-produced SWE grids with reference data from the Canadian database CanSWE, and GMON stations, which measure SWE using gamma ray attenuation. This study also compares the UdeS grids with four other gridded databases that are widely used in hydrology: ERA-5 Land, SNODAS, MERRA and Crocus-ERA-5. Three indices are used to evaluate the ability of these databases to estimate the duration of the snow cover period: the start and end dates of snow cover and the start date of snowmelt. The annual maximum of SWE, the correlation coefficient, bias, and root mean square error (RMSE) are other indices used to evaluate the ability of these databases to estimate SWE values. The main results show that, despite some differences, particularly in the north-eastern part of the study area, all databases accurately estimated the duration of the snow cover period. Except for the MERRA database, which appears to underestimate the SWE in our study area, the results show that all databases perform well. ERA-5 Land appears to perform better, although it overestimates the reference data. UdeS and Crocus perform similarly but underestimate the reference data.

How to cite: Bathelemy, R., Boucher, M.-A., Redondo Tilano, S. A., and Hamelin, J.: Evaluation of the performance of a database for snow water equivalent in southern Quebec, obtained using a spatialised particle filter, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6027, https://doi.org/10.5194/egusphere-egu26-6027, 2026.

EGU26-6555 | ECS | Posters on site | HS2.1.4

Recent Trends in Snow Water Equivalent and Evapotranspiration in the Western Italian Alps: Emerging Signals of Climate Warming 

Alessio Gentile, Davide Gisolo, Tanzeel Hamza, Aurora Olivero, Matteo Salis, Aqsa Aqsa, Stefano Bechis, Stefano Ferrari, Davide Canone, and Stefano Ferraris

European Alps are essential sources of water sustaining downstream ecosystems and human activities. In this regard, they are referred to ‘the water towers of Europe’. However, these regions are also among the most sensitive to climate change. Indeed, the high rate of temperature increase, altered precipitation regimes, and “snow droughts”, i.e., a lack of snow accumulation in winter, are significantly impacting the hydrological processes in snow-dominated areas.

In this context, Snow Water Equivalent (SWE) and Actual EvapoTranspiration (AET) are two key variables for understanding the mountain water cycle. Investigating SWE and AET changes is essential to detect whether the hydrological cycle is accelerating in response to climate warming.

Gridded datasets, such as those derived from reanalysis products or satellite-based observations, have significantly enhanced the spatial representation of climatic and environmental variables in topographically complex regions, where the availability of ground-based observational data is often sparse or unevenly distributed due to logistical and environmental constraints.

This study examines the dynamics of SWE and AET over recent years across catchments of varying spatial scales in the Western Italian Alps, based on SWE data from the IT-SNOW dataset and AET data from MODIS. The analysis also includes a comparison between gridded data and in-situ measurements. The main aims are:

  • evaluate the ability of gridded datasets to capture key hydrological processes at multiple spatial scales;
  • identify shifts in snow regimes and evapotranspiration patterns potentially driven by climate warming;
  • assess the reliability of gridded data for local-scale hydrological applications through comparison with ground-based observations.

This publication is part of the project NODES which has received funding from the MUR – M4C2 1.5 of PNRR funded by the European Union - NextGenerationEU (Grant agreement no. ECS00000036). This work was supported  by the PRIN 2022 202295PFKP SUNSET Project and by Funding 2023-2025 Fondazione CRT.

How to cite: Gentile, A., Gisolo, D., Hamza, T., Olivero, A., Salis, M., Aqsa, A., Bechis, S., Ferrari, S., Canone, D., and Ferraris, S.: Recent Trends in Snow Water Equivalent and Evapotranspiration in the Western Italian Alps: Emerging Signals of Climate Warming, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6555, https://doi.org/10.5194/egusphere-egu26-6555, 2026.

EGU26-7317 | ECS | Orals | HS2.1.4

High-Altitude Himalayan Meltwater Contributions Revealed by Isotopic Analysis 

Benjamin Graves, Tom Matthews, and Richard Taylor

Melting glaciers provide crucial seasonal water to communities in high mountain regions. To project how mountain water resources will be impacted by glacial recession requires quantification of current contributions of glacier meltwater to streamflow. This is particularly challenging in monsoon-affected regions, where high glacier melt rates are synchronous with very high precipitation rates. Glacio-hydrological modelling provides a way of estimating meltwater contributions, but confidence in applied conceptual and numerical models is enhanced by observations. Here, stable isotope ratios of oxygen and hydrogen are employed in order to trace relative contributions of multiple sources to the flow of the Dudh Koshi river in northeastern Nepal. Integration of 45 new observations from river, glacial melt, and snow samples with 784 previous observations creates a comprehensive multi-season dataset; these data constrain a mixing model to resolve contributions to river flow that vary seasonally and along the river transect. Preliminary results from the new post-monsoon samples indicate the highest meltwater fractional contribution yet seen in this region.

How to cite: Graves, B., Matthews, T., and Taylor, R.: High-Altitude Himalayan Meltwater Contributions Revealed by Isotopic Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7317, https://doi.org/10.5194/egusphere-egu26-7317, 2026.

EGU26-8202 | ECS | Orals | HS2.1.4

Elevation-dependent snow cover changes across Switzerland in the 21st century 

Harsh Beria, Sven Kotlarski, Adrien Michel, Tobias Jonas, and Christoph Marty

Snow provides numerous ecosystem and economic services, such as hydropower generation, regulation of stream temperature, and winter tourism. Despite projected increases in winter precipitation, warming temperatures are expected to reduce snowfall and shift precipitation toward rainfall, fundamentally changing snowpack accumulation dynamics, and the associated hazards such as rain-on-snow flooding. This highlights the need for accurate snow projections at locally relevant spatial scales.

Here, we present novel high-resolution (1x1 km²) daily projections of snow water equivalent (SWE) and snow depth for Switzerland, based on the recently released Climate CH2025 scenarios. SWE is simulated for an ensemble of 12 bias-adjusted regional climate models from the EURO-CORDEX initiative using a distributed temperature-index snow model, which is statistically nudged toward a reference SWE dataset (SPASS) – derived from the same model but debiased using data assimilation with observations from 1998-2024.

We project widespread SWE declines across Switzerland, with the largest percentage reductions at low elevations (<1000 m a.s.l.), and a transition from seasonal to ephemeral snowpacks at intermediate elevations. We further assess the added value of high-resolution snow simulations by comparing them with physically-based, but coarser (~12 km) raw EURO-CORDEX SWE projections. While both show consistent large-scale patterns, our higher resolution simulations reveal clearer elevation-dependent signals, especially in topographically complex mountainous landscapes, enabling robust estimation of locally relevant snow indicators. These results offer actionable insights for managing future snow-dependent resources in a rapidly warming climate.

How to cite: Beria, H., Kotlarski, S., Michel, A., Jonas, T., and Marty, C.: Elevation-dependent snow cover changes across Switzerland in the 21st century, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8202, https://doi.org/10.5194/egusphere-egu26-8202, 2026.

EGU26-9801 | ECS | Orals | HS2.1.4

Improving the spatial distribution of snow height in physics-based snow models using large-area airborne lidar-scans 

Jens Oprel, Jan Magnusson, Tobias Jonas, Manuela Brunner, Karoline Holand, Andreas Stordal, and Gaute Lappegard

Predicting the volume and timing of snowmelt is essential for applications such as hydropower production planning and flood forecasting. The timing of snowmelt is strongly influenced by the spatial distribution of snow. A more heterogeneously distributed snowpack leads to a longer melt season and lower peak flow than a homogeneously distributed snowpack. Despite the importance of spatial snow distribution for runoff characteristics, large-scale and high-resolution measurements of snow distribution are rare and it is challenging to effectively use such measurements in models when the snow conditions differ substantially across the study region.

We acquired high-resolution airborne lidar snow height maps in three winters for three large hydropower regions in Southern Norway, covering over 1000 km2. We use these to improve snow height simulations and demonstrate how the scans can be assimilated into a physics-based snow model. To this end, we use a snowfall scaling method that aims to implicitly describe preferential deposition and redistribution processes during snow accumulation by altering the snowfall inputs to the snow model. In each grid cell, a scaling factor is chosen such that the modelled snow height matches the observed snow height. Existing methods are often not finding the optimal scaling factor, especially in case snowmelt has started in parts of the scanned regions. We present a new approach that considers estimated snow losses due to melt and sublimation that occurred before the acquisition of the lidar scan. With this improvement, scans taken slightly after melt onset in part of the region can still be used to reliably find the optimal snowfall scaling factors, even if part of the snow is already lost due to melt and sublimation.

We show how similar these snowfall scaling factors are between years, due to repeatable patterns in snow height, and whether this similarity provides opportunities to transfer snowfall scaling factors to different years. Furthermore, we show that higher model resolutions are best suited to represent the observed spatial snow distribution in the model using the proposed snowfall scaling method. The insights of this work can be used to effectively use large area, high-resolution snow height measurements in snow models.

This work is partially funded by Statkraft Energi AS and the Norwegian Research Council (SnowInflow, NFR 346308).

How to cite: Oprel, J., Magnusson, J., Jonas, T., Brunner, M., Holand, K., Stordal, A., and Lappegard, G.: Improving the spatial distribution of snow height in physics-based snow models using large-area airborne lidar-scans, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9801, https://doi.org/10.5194/egusphere-egu26-9801, 2026.

Quantifying snow water equivalent (SWE) and melt dynamics across the Pan-Siberian domain is critical for understanding the hydro-climatological conditions of the entire Northern Hemisphere. However, due to the scarcity of data, the strong interaction between vegetation and climate, and representativeness biases of sparsely distributed measurement stations, there is a high degree of uncertainty in current estimations. While traditional monitoring networks provide essential points of reference, their limited spatial coverage and site-selection biases—often favoring open clearings—hinder the accurate assessment of regional snow storage across diverse and complex landscapes.
In this study, we develop and apply a physics-based snow process model designed for data-sparse cold regions, combined with a corresponding regionalization strategy to bridge the gap between sparse point-scale observations and regional snow dynamics. The model was first validated at the Sodankylä site in Finland, demonstrating high performance for both Snow Depth (NSE > 0.78) and SWE (NSE > 0.83), indicating a physically consistent representation of snow density, compaction, and melt processes. The model was then applied across Pan-Siberia by grouping 85 stations into hydro-climatic regimes based on wind, precipitation characteristics, and forest cover. Model parameters were calibrated simultaneously across stations within each regime to derive robust zonal parameter sets, thereby ensuring physical consistency and overcoming parameter equifinality.
The resulting regionalized model achieves robust performance across the majority of the domain (median KGE > 0.75), substantially outperforming global default parameterizations. The results reveal a key physical insight in forest-dominated Taiga regions, where the optimized wind correction factor converges toward zero, confirming the strong canopy sheltering effect and indicating that standard WMO wind corrections systematically overestimate snowfall under forest cover. In contrast, the Cold Continental regime (Yakutia) exhibits a high rain–snow temperature threshold (~+3.7°C), reflecting sublimation-driven cooling under extremely dry atmospheric conditions. 
This approach enables the reconstruction of spatially consistent, multi-year snow dynamics across Pan-Siberia, providing a scalable strategy for hydrological modeling in ungauged, cryosphere-dominated regions and offering new insights into the spatiotemporal evolution of Eurasian snow resources.

How to cite: Luo, J. and Menzel, L.: A Physics-Based Regionalized Snow Modeling Framework for the Data-Sparse Pan-Siberian Domain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9883, https://doi.org/10.5194/egusphere-egu26-9883, 2026.

EGU26-10888 | Orals | HS2.1.4

Assessment of snow model uncertainty using a large number of openAMUNDSEN snow model configurations: A study from the Berchtesgaden National Park (Germany) 

Erwin Rottler, Brage Storebakken, Michael Warscher, Florian Hanzer, Elena Bertazza, and Ulrich Strasser

While the assessment of climate model uncertainty is well established, the uncertainty originating from the selection of a surface snow model usually only receives little attention. However, a better understanding of snow model uncertainty currently becomes more and more important, as novel climate model data at the kilometer-scale, innovative downscaling techniques, and increasing computational capacities are among the elements that pave the way for a new phase of high resolution and physically based climate change impact studies assessing cryospheric changes in complex mountain areas. To investigate the uncertainty induced by the selection of the snow model configuration, we simulate the seasonal snow cover in the mountain area of the Berchtesgaden National Park (Germany) under historical conditions (10/2013 - 09/2023) and for a 10-year period characterized by a 1°C warming. Therefore we use a large number of openAMUNDSEN snow model configurations (n = 108) with T-Index, enhanced T-Index as well as energy balance based snowmelt methods, varying land cover maps and spatial resolutions. Forcing data for the 10-year warming period is constructed using the stochastic bootstrap resampler (climate generator) available within the openAMUNDSEN modelling framework. Prior to the estimation of snow model uncertainty, we evaluate the snow model results using satellite-based snow data. Our results suggest that differences in key snow metrics such as snow cover duration and snow disappearance day can be in the same range as the impact of a 1°C warming. The results also support the identification of critical snow model settings that need to be considered, in particular, when using energy balance instead of degree-day snow models to investigate climate change impacts on snow hydrological processes in complex mountain terrain.

How to cite: Rottler, E., Storebakken, B., Warscher, M., Hanzer, F., Bertazza, E., and Strasser, U.: Assessment of snow model uncertainty using a large number of openAMUNDSEN snow model configurations: A study from the Berchtesgaden National Park (Germany), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10888, https://doi.org/10.5194/egusphere-egu26-10888, 2026.

EGU26-11091 | Orals | HS2.1.4

Global glacier contribution to streamflow 

Fanny Brun, Marit van Tiel, Matthias Huss, and Giulia Mazzotti

Glacier contribution to streamflow has mostly been investigated at the scale of relatively small catchments, and more rarely at the scale of the major rivers. In this study, we compare monthly glacier mass changes to monthly estimates of streamflow for the period 1990-2023, both annually and seasonally for 55 major river basins larger than 5700 km2 (0.01 to 20.0 % glaciated). Monthly mass changes for every individual glacier are obtained by temporally downscaling geodetic elevation change observations with the variability from in situ glaciological measurements and global-scale model results. Streamflow is based on GLOFAS and G-RUN global datasets. GLOFAS is a land surface model forced by ERA5 reanalysis that feeds a channel routing model. G-RUN is a machine learning algorithm that predicts monthly runoff based on the Global Soil Wetness Project Phase 3 dataset. Basin scale precipitation and evapotranspiration are estimated from ERA5 reanalysis data.

Annual glacier mass change and thus water release ranges from near zero to 550 mm at the basin-scale and roughly correlates with the percentage of the glacierized area in the basin.  The ratio of annual glacier mass change divided by the mean annual discharge, hereafter called the annual glacier contribution, is below 6 % for all the basins larger than 500’000 km2, with the exception of the Indus river with an annual glacier contribution of 25 % (40 mm). The Indus river basin is both highly glacierized (more than 3 %) and arid, explaining such a high ratio.

The glacier seasonal contributions, defined as the water volume derived from glacier mass change during summer months (JJAS in the northern hemisphere and DJFM in the southern hemisphere), divided by the mean discharge in the same months, are always higher than the annual ones. In particular for the basins with low flow during the melt season (e.g. Rapel, Skagit, Rhone, Columbia, Biobio, Po, Rhine), the seasonal contribution is more than three times the annual one. On average 62 % of the glacier mass change originate as a balance contribution, meaning that it corresponds to the seasonal snow accumulation. In contrast, 38 % of the glacier contribution originates from ice melt, i.e. the unsustainable release of the solid water stored in glaciers.

Besides uncertainties in glacier mass change and streamflow data, evaporation (of the glacier meltwater) and groundwater contributions are not treated explicitly, which might lead to overestimations of the glacier contributions. It should thus be seen as a first-order estimate that highlights the major contrasts between basins at the global scale.

How to cite: Brun, F., van Tiel, M., Huss, M., and Mazzotti, G.: Global glacier contribution to streamflow, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11091, https://doi.org/10.5194/egusphere-egu26-11091, 2026.

EGU26-11618 | ECS | Posters on site | HS2.1.4

From Snow to Rain: Elevation-Dependent Drought Responses and Drivers in a Large Italian Alpine Catchment. 

Senna Bouabdelli, Martin Morlot, Christian Massari, and Giuseppe Formetta

Drought has recently emerged as a common hazard in Alpine regions, where snow
dynamics strongly influence river flow regimes and play a crucial role in reservoir filling,
irrigation, tourism, and ecosystem sustainability. Reduced snow contributions and
warmer winters, which enhance rainfall at the expense of snowfall, can shift the
hydrological behaviour of Alpine catchments toward regimes typical of lower elevations.
In this study, we assess the main drivers of drought in the Adige River basin, a large
Italian Alpine basin characterized by sub-catchments spanning a wide range of
elevations over the period (1980-2018). We further investigate the seasonality and
characteristics of drought events across elevation bands to identify the drought types
with the greatest impacts in terms of total severity and duration. Our results show that
cold-season snow drought is the dominant drought type over the study period, followed
by snowmelt drought and rainfall deficit drought. Mid- and high-elevation sub-
catchments are particularly affected by cold season and snowmelt drought, whereas
low-elevation areas are mainly impacted by rainfall deficit drought. These findings
highlight the need for adaptation strategies that explicitly account for seasonal drought
processes and elevation-dependent river responses to sustain mountain water systems
under increasing drought conditions, especially given the implications for hydropower
production, irrigation, and tourism.

How to cite: Bouabdelli, S., Morlot, M., Massari, C., and Formetta, G.: From Snow to Rain: Elevation-Dependent Drought Responses and Drivers in a Large Italian Alpine Catchment., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11618, https://doi.org/10.5194/egusphere-egu26-11618, 2026.

EGU26-13523 | Posters on site | HS2.1.4

Sentinel-2 Based Validation of Snow Covered Area of Alpine3D Simulations Applying Snow Depth Pattern Redistribution across Two High-Alpine Karst Catchments 

Roberta Facchinetti, Elias Bögl, Paul Schattan, Jakob Knieß, Karl-Friedrich Wetzel, Karsten Schulz, and Franziska Koch

Modelling high-alpine hydrology poses significant challenges due to terrain heterogeneity and complex topography. In snow-dominated karst catchments, accurate representation of spatiotemporal snow distribution is essential for simulating aquifer recharge and spring discharge dynamics. However, differences in data availability and landscape complexity can be a limit. Here, we assess the ability of Alpine3D applying snow pattern redistribution to capture the spatiotemporal snow cover variability in two adjacent alpine karst catchments with different spatial snow distribution characteristics.

We present an 11-year (2015-2025) validation of Alpine3D simulations in two adjacent high-alpine karst catchments in the Zugspitze region in Germany (European Alps): the Partnach Spring catchment (15.4 km², 1430-2962 m a.s.l.) and the Hammersbach catchment (17.8 km², 768-2951 m a.s.l.). While both catchments share similar karstified alpine geomorphology, Partnach Spring is characterized by higher elevations on average, limited vegetation, and more persistent snow cover, whereas Hammersbach exhibits stronger elevation gradients, greater forest cover, and higher radiation exposure, leading to more heterogeneous snow accumulation and melt dynamics.

Precipitation and snow were redistributed in order to correct snow water equivalent quantitatively and spatially. Therefore, we used a snow depth map derived by Pléiades stereo satellite images taken on the 9th of April 2021, near peak snow accumulation. Data gaps, e.g. due to shaded areas and very steep terrain were filled using Random Forest trained on terrain attributes, topographic indices, and energy balance parameters. Alpine3D was run at 16 m × 16 m resolution with spatially interpolated meteorological station data on an hourly base and was validated against Sentinel-2 snow cover area (SCA) maps during the melt season (May-August). Snow classification employed dual thresholds (red band reflectance and NDSI) with manual cloud masking and DEM-based shadow removal. Modelled performance was evaluated using pixel-based confusion matrices across multiple dates per year, whereof we will present preliminary results for both catchments.

This multi-catchment approach with different characteristics, but similar meteorological conditions aim to demonstrate the transferability of this snow redistribution method across different alpine environments. The results are valuable insights for improving hydrological predictions in ungauged basins with limited spatially distributed snow observations.

How to cite: Facchinetti, R., Bögl, E., Schattan, P., Knieß, J., Wetzel, K.-F., Schulz, K., and Koch, F.: Sentinel-2 Based Validation of Snow Covered Area of Alpine3D Simulations Applying Snow Depth Pattern Redistribution across Two High-Alpine Karst Catchments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13523, https://doi.org/10.5194/egusphere-egu26-13523, 2026.

EGU26-13824 | ECS | Posters on site | HS2.1.4

A Methodological Framework for Harmonized Comparison of Model-Based and Satellite-Derived Snow Cover Products in Data-Sparse Mountain Regions of Kyrgyzstan.  

Jumana Akhter, Beatrice Marti, Peter Molnar, Joel Caduff-Fiddes, and Silvan Ragettli

In the glacier-melt-dominated regions of Kyrgyzstan, accurate cryosphere monitoring is essential for Central Asian water resource forecasting. However, the lack of consistent in situ observations necessitates the integration of diverse remote sensing datasets and physically based models which often vary in their underlying assumptions and resolutions. This study presents a transparent, reproducible framework for the comparative evaluation of heterogeneous snow products in complex terrain, applied to SnowMapper (a NWP-driven physical model) and GlacierMapper (a MODIS-based NDSI product) for the period 2000–2024.

The framework employs spatial harmonization via nearest-neighbor resampling to a common independent grid and temporal alignment across differing calendar conventions. To address variable incompatibility, Snow Water Equivalent (SWE) outputs from SnowMapper are transformed into binary snow/no-snow classifications using literature-derived thresholds. Sensitivity analyses reveal that product agreement is significantly influenced by these methodological transformations. Evaluation using complementary spatiotemporal diagnostics such as fractional snow cover area, balanced accuracy, Cohen’s kappa and snow depletion curves (SDCs) identifies periods of systematic divergence across decadal and seasonal timescales. Results demonstrate that apparent product discrepancies arise not only from physical inconsistencies but also from methodological treatment. This standardized intercomparison approach is transferable across sensors and regions enhancing the reliability of snow-product assessments in data-scarce mountain environments.

How to cite: Akhter, J., Marti, B., Molnar, P., Caduff-Fiddes, J., and Ragettli, S.: A Methodological Framework for Harmonized Comparison of Model-Based and Satellite-Derived Snow Cover Products in Data-Sparse Mountain Regions of Kyrgyzstan. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13824, https://doi.org/10.5194/egusphere-egu26-13824, 2026.

EGU26-14610 | ECS | Posters on site | HS2.1.4

Process-based modelling of the energy and water balance of the Rio Santa Basin, Peruvian Andes 

Yota Sato, Catriona Fyffe, Thomas Shaw, Vinisha Varghese, Achille Jouberton, Maximiliano Rodriguez, and Francesca Pellicciotti

Glaciers in the Peruvian Andes play a crucial role in sustaining regional water resources for downstream populations and ecosystems, have been experiencing rapid mass loss and retreat in recent decades. The region is characterised by a tropical semi-arid climate with minimal seasonal temperature variability, alternating dry and wet seasons, and high-elevation areas frequently experience air temperatures close to 0 °C. These conditions lead to dynamic glacier energy-balance processes, in which intermittent and ephemeral snow strongly controls melt. Furthermore, these glacierized areas provide water resources to fragile downstream ecosystems, as well as subsistence and commercial agricultural systems, which themselves alter the water balance. It is challenging to reproduce the energy and water balance of such a complex environment using simplified, empirically parameterised models, and integrated, process-based modelling approaches might offer a viable way forward under a changing climate. We use a physically-based land surface modelling framework to disentangle the spatio-temporal variability of the energy and water balance of a large catchment in the Peruvian Andes. 

Within this study we focus on the Rio Santa basin (4950 km2), located in the Cordillera Blanca, which contains ~330 km2 of glacier area at elevations of 4300-6300 m a.s.l. We employ the process-based land-surface model Tethys-Chloris to simulate energy and water fluxes over a 9-year period (2010-2018) for the whole catchment. We use downscaled meteorological forcing derived from a WRF climate model simulation forced by ERA5 reanalysis. Meteorological forcings are bias-corrected using observations from multiple automatic weather stations across the catchment. The model is evaluated using in-situ glacier observations, including mass balance, surface albedo, and snow-pit measurements, as well as remote-sensing products covering the catchment. 

We present a comprehensive, process-based simulation of the catchment-scale water balance of the Rio Santa basin. We quantify the altitudinal distribution and the spatial, seasonal, and interannual variability of the blue-green-white water balance and its individual components across the entire catchment. We further estimate the energy- and mass-balance components of all glaciers in the Cordillera Blanca (445 glaciers) to identify hotspots of glacier changes and their controls. This allows us to determine the importance of sublimation for controlling glacier mass balance and the role of ephemeral snow in shaping melt rates. A key step forward is the catchment-wide quantification of catchment losses, where we identify the combined role of sublimation and evapotranspiration in the water balance. These results provide a novel process-based understanding of the energy and water balance of the Rio Santa basin to establish a mechanistic baseline simulations to understand future changes in the system.

How to cite: Sato, Y., Fyffe, C., Shaw, T., Varghese, V., Jouberton, A., Rodriguez, M., and Pellicciotti, F.: Process-based modelling of the energy and water balance of the Rio Santa Basin, Peruvian Andes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14610, https://doi.org/10.5194/egusphere-egu26-14610, 2026.

EGU26-14775 | ECS | Posters on site | HS2.1.4

Assessing climate change impacts on pristine glaciated catchments in the Alpine region using indicators of hydrological alteration 

Chahinaz Ziani, Lars Ribbe, Moritz Heinle, Renee van Dongen-Köster, Claudia Zentis, Tinh Vu, and Luna Bharati

Glaciers sustain the global water cycle and preserve natural ecosystems by acting as reservoirs that release consistent freshwater during dry periods. This meltwater supports biodiversity, nutrient balances, river streamflow modulation, and human activities such as irrigation and water supply. Currently, accelerating glacier melt has become an alarming phenomenon, with global glacier mass loss of around 5% since 2000. This contributes to sea-level rise and threatens water supplies for over 2 billion people. In this context, this study aims to assess the impacts of climate change on pristine glaciated catchments in the Apline region, where accelerating ice loss threatens spring and summer river flows that are vital for ecosystems and societies. Using the ROBIN dataset, we calculated seasonal (i.e., spring and summer) indicators of hydrologic alterations (magnitude, timing, extremes) comparing pre-climate change (1931–1950) and post-climate change (1977–2012) baselines for 20 pristine catchments with areas ranging between 22 Km2 -981 Km2.

Results in spring and summer reveal high variability in key flow indicators (including mean monthly and seasonal flows, rise and fall rates, In addition to  seasonal minimum and maximum flows) especially across the six largest catchments in the study area (> 345 Km2). Comparing the post-climate change period (1977–2012) to the pre-climate change baseline, results indicated increased interquartile ranges and greater uncertainty of mean values associated with seasonal flow rates. Additionally, they showed irregular occurrences of extremes regarding their timing, frequency, and duration of high and low pulses, as well as flow reversals, for all catchments. These findings indicate increased dispersion, extremes, and instability associated with a meltwater buffer zone.

These results highlight that climate change has a strong impact on pristine Alpine glaciated catchments with limited human intervention, showing how increased glacier melting rates trigger hydrological fluctuations with pivotal implications on water resources management. This situation requires effective adaptation measures concerning increased ice melting rates.

How to cite: Ziani, C., Ribbe, L., Heinle, M., van Dongen-Köster, R., Zentis, C., Vu, T., and Bharati, L.: Assessing climate change impacts on pristine glaciated catchments in the Alpine region using indicators of hydrological alteration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14775, https://doi.org/10.5194/egusphere-egu26-14775, 2026.

EGU26-15976 | ECS | Orals | HS2.1.4

Tree sway monitoring for improved representation of canopy snow interception in cold, wet climates 

Emmanuelle Barrette, Vincent Vionnet, Benjamin Bouchard, and Daniel F. Nadeau

In cold and wet regions, the forest canopy strongly influences the energy and mass balance of the snowpack by intercepting a large fraction of solid precipitation. Although commonly represented in land-surface models, snow interception remains poorly documented in the field because of the difficulties associated with directly measuring intercepted snow mass. Existing indirect measurement approaches include the use of accelerometers to quantify wind-induced tree sway and relate changes in sway frequency to variations in intercepted snow mass. However, this experimental method has so far been applied at only one site in the western United States, under climatic conditions that differ from those of the boreal forests of eastern Canada.

The objective of this study is to apply the tree sway method in eastern Canada to estimate intercepted snow mass and to improve the parametrization of canopy snow interception in the SVS2–Crocus land surface model.

A total of nine coniferous trees were equipped with accelerometers across three sites to monitor wind-induced tree sway and obtain estimates of intercepted snow mass. Results from the winter 2024–25 show that the sway method captures rapid loading and unloading events, with sway frequency responding to interception and release within a few hours, in agreement with hourly timelapse imagery acquired at each site. The resulting intercepted snow time series is then used to evaluate the canopy interception parametrization in the SVS2–Crocus model, which was forced using in situ meteorological measurements.

Sway-based observations and simulated intercepted snow mass show good agreement in the timing of interception and unloading, with rapid increases during snowfall and subsequent exponential decay. However, the model tends to overestimate slow, continuous unloading and often fails to accurately reproduce rapid unloading events associated with strong winds, warm temperatures, or rain-on-snow events. These results pave the way for improving the parametrization of canopy snow unloading in SVS2–Crocus and, in turn, for more accurately estimating snow cover in forested environments.

How to cite: Barrette, E., Vionnet, V., Bouchard, B., and Nadeau, D. F.: Tree sway monitoring for improved representation of canopy snow interception in cold, wet climates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15976, https://doi.org/10.5194/egusphere-egu26-15976, 2026.

EGU26-16472 | ECS | Posters on site | HS2.1.4

Most Asian Glaciers Will Deplete After Mid-Century: Linking Mass Loss to Peak Water Runoff 

Muhammad Mannan Afzal, Xie Fuming, and Shiyin Liu

Glacier runoff in High Mountain Asia (HMA) is approaching peak water in many regions, with asynchronous timing across basins due to differences in glacier size, elevation, and climate forcing. Using the Open Global Glacier Model (OGGM v1.6.1), we simulate glacier mass balance (1940–2019), glacier dynamics and runoff (1940–2100) across 17 major basins, driven by bias-corrected GSWP–W5E5 historical forcing and an ensemble of 13 CMIP6 GCMs and four SSP scenarios. Small, low-elevation glaciers have already surpassed their peak runoff and are rapidly vanishing, whereas large, high-elevation glaciers continue to buffer downstream flows into the late 21st century particularly in glacier-rich basins such as the Indus and Tarim. HMA-wide glacier mass is projected to decline by 57–82% between 2001-2100, accompanied by an overall 10 ± 6.5% reduction in glacier runoff. Crucially, basin-scale hydrological shifts are not dictated by average glacier behavior, but by the composition and distribution of glacier classes. Clustering analysis reveals three distinct peak-runoff regimes, early, transitional, and delayed primarily controlled by glacier size, elevation, and regional climate. These staggered peak-runoff patterns highlight pronounced spatial heterogeneity in HMA’s hydrological response and underscore the urgency of basin-specific adaptation strategies in one of Earth’s most densely populated and climate-sensitive mountain regions.

How to cite: Afzal, M. M., Fuming, X., and Liu, S.: Most Asian Glaciers Will Deplete After Mid-Century: Linking Mass Loss to Peak Water Runoff, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16472, https://doi.org/10.5194/egusphere-egu26-16472, 2026.

Southeast Alaska represents a highly variable hydrologic environment. Headwaters are dominated by alpine glaciers and larger river basins envelop significant glacier area. Daily estimates of streamflow and river temperature provide useful insight into regions undergoing rapid change. Here we present a river temperature model framework that adapts results from two different streamflow models applied in Southeast Alaska. We compare streamflow inputs from two land surface models: 1) a coupled simulation of RASM-CTSM at 4 km and 2) an offline run of RASM-WRF Hydro Glacier at 1 km. The land surface models primarily differ in glacier treatment, RASM-CTSM uses a traditional five-layer snow model to account for changes to glacier processes, while the RASM-WRF Hydro Glacier model applies the dynamic CROCUS snow model for improved glacier simulations in river basins with glacier presence. The RASM-WRF Hydro Glacier employs the three-layer snow model from the NoahMP land surface component to account for non-glaciated basins. Runoff from both models is routed to streamflow and the River Basin Model (RBM) is used to produce daily river temperature data. The models were run for a historical (1991-2020) period, including a parameter sensitivity test for river temperature, and then applied to a mid-century (2035-2064) climate scenario. We validated the river discharge and temperature estimates against USGS observations at seven basins. We assess model performance in terms of the Kling-Gupta Efficiency metric and its three components, correlation, volume bias, and variance bias. We also assess an overall percent bias between modeled and observed data.  In historical simulations, the RASM-WRF Hydro Glacier performs better than the RASM-CTSM model across all metrics in glaciated basins, while producing identical results in non-glaciated basins, indicating that the RASM-WRF Hydro Glacier model produces more accurate results and should be employed for future simulations. Estimates of future changes in discharge and stream temperature, together with glacier contributions to runoff, provide a holistic assessment of hydrologic system change in Southeast Alaska, useful for land management. The results provide the baseline for future investigations and modeling studies of the impacts of projected changes on fish habitats and hydrological trends in this glacier-dominated landscape.

How to cite: Gilbert, C. and Musselman, K.: Comparing the Impact of Differing Glacier Contribution Assessments on Modeled Discharge and River Temperature Across Southeast Alaska, USA, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16527, https://doi.org/10.5194/egusphere-egu26-16527, 2026.

EGU26-16647 | Orals | HS2.1.4 | Highlight

The changing water cycle of the mountains 

Francesca Pellicciotti, Mike McCarthy, Achille Jouberton, Alvaro Ayala, Catriona Fyffe, Maximiliano Rodriguez, Pascal Buri, Thomas Shaw, Adria Fontrodona Bach, and Zhenya Tumarkin

Much of the freshwater sustaining human societies is generated in the mountains: the mountain cryosphere supports almost a third of the global population for irrigation, drinking water, industry and the environment. At the same time, this crucial resource is undergoing unprecedented changes, with glaciers shrinking, snow decreasing globally and permafrost thawing across continents. This bigger picture masks a very large variability of responses across climates and continents, shaped by processes specific to different mountain ranges. Glaciers and seasonal snow are often assumed to respond to a changing climate in a linear manner, especially at large and global scales, given the complexity of interactions among them and the eco-hydrology of the catchments they sustain. Growing evidence suggests more complex dynamics and threshold effects that will affect the water resources they generate. 

In this talk, I will focus on processes and non-linearities in the mountain cryosphere that shape the mountain water cycles across climates, and show how that water cycle is changing  across regions as a result. I will focus on a number of specific processes: i) the role of ephemeral and marginal snowpacks on streamflow generation, and their vulnerability to temperature and precipitation shifts, especially in sub-tropical regions; ii) changes in precipitation phase, and their distinct effects on the water cycle depending on precipitation seasonality; iii) the transition from sublimation to melt in a warmer world and how that can change the assumed linear trajectory of water from glaciers and snow in arid areas; iv) the role of evaporative fluxes in the mountain water cycle and how warming promotes increased evapotranspiration that recycle increasing portions of high-altitude precipitation and surface water into the atmosphere. Another key disruption in the functioning of mountain systems is the increasing frequency and intensity of droughts, and I will show some very recent results about how glaciers buffer droughts, and how this capacity might be hampered when droughts become more severe and of longer duration. We use for most of these investigations a fully mechanistic, physically-based modelling framework that represent both the cryosphere, the biosphere and hydrosphere of mountain regions, and I will also briefly touch on the modelling strengths and limitations. 

Our results show that the response of the cryosphere to ongoing changes in the climate is very heterogenous. Ephemeral snow in sub-tropical, semi-arid climates has been mostly neglected in modelling assessments, invisible to satellite images, but represents the main contributor to water runoff, and yet this will change in the future with increasing temperatures, which will remove a major source of water. Overall, shifting snowline altitudes and shrinking accumulation areas will move the areas of water generation to higher elevations, altering storage and routing patterns and seasonality, and accelerating the water cycle. Droughts are changing the functioning of mountain systems, with evapotranspiration amplifying water deficits in many mountain regions, while snow droughts enhance this so-called drought paradox. I will conclude with a perspective of future research on mountain processes and water resources. 

How to cite: Pellicciotti, F., McCarthy, M., Jouberton, A., Ayala, A., Fyffe, C., Rodriguez, M., Buri, P., Shaw, T., Fontrodona Bach, A., and Tumarkin, Z.: The changing water cycle of the mountains, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16647, https://doi.org/10.5194/egusphere-egu26-16647, 2026.

Seasonal snowmelt strongly influences hydrological and ecological processes by controlling the timing of peak soil moisture and subsequent vegetation growth; yet, this relationship is less studied in the Indian Himalayan region, especially in Himachal Pradesh’s snow region. This study investigates the linkage between snow disappearance timing and peak soil moisture using station data across various elevation ranges from 1571 m to 3325 m and the FLDAS dataset (daily, 0.01° resolution), and then their effect on vegetation growth using the MODIS NDVI product (8-day, 250-m resolution). We quantified the spatial and temporal variability in snow recession by fitting an exponential decay model. The recession rate varies between 0.03 and 0.27 across various elevation ranges and temporal periods. The recession rate also exhibits a strong elevation dependency, being low at higher elevations (e.g., Lari, 3325 m m.s.l., k = 0.044 m/day) and high at lower elevations (e.g., Dodra Kawar, 2522 m m.s.l., k = 0.169 m/day). Based on analysis from 2001 to 2020 across nine stations, results show that snow onset occurs in mid-December, followed by snow recession in late February and complete snow disappearance by late March across Himachal Pradesh. We observed an average lag of 3-4 days between the timing of peak soil moisture and snow disappearance, and a correlation of 0.94 (p < 0.05) was observed across various stations. Early melt does contribute to greening, as evidenced by the weaker but still positive correlation (0.54, p < 0.05) between the timing of snow disappearance and the rise in NDVI. The results show that the timing of snowmelt primarily influences soil moisture dynamics and controls vegetation activity in Himalayan catchments.

How to cite: Nanda, A., Bharti, A., and Varade, D.: Understanding the Role of Snowmelt Processes on Soil Moisture Storage and Vegetation Dynamics acrossTopographic Gradients of Himalayan Catchments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16655, https://doi.org/10.5194/egusphere-egu26-16655, 2026.

EGU26-16791 | ECS | Orals | HS2.1.4

Dynamic identification of snow phenology in the Northern Hemisphere 

Le Wang, Xin Miao, and Weidong Guo

Snow phenology characterizes the cyclical changes in snow and has become an important indicator of climate change in recent decades. Changes in snow phenology can significantly impact climate and hydrological conditions. Previous studies commonly employed fixed threshold methods to extract snow phenology. However, these methods do not account for the variability in snow distribution across the Northern Hemisphere, leading to potential biases of snow phenology. In this study, we observe that snow phenology extracted from different snow data and methods shows significant differences, but consistently underestimates snow duration at low and middle latitudes. Our analysis further indicates that the changes in snow depth exhibits a significant shift around 10% of peak value across the Northern Hemisphere, marking the transition between the snow and non-snow seasons. We further apply the 10% snow depth threshold and investigate the differences between original and newly extracted snow phenology. At low and middle latitudes, the snow cover duration (SCD) extends, the snow cover onset day (SCOD) advances, and the snow cover end day (SCED) delays, especially on the Tibetan Plateau, where the SCD differences can reach 28 days. The change at higher latitudes is reversed. The dynamic snow phenology accounts for the spatial heterogeneity of Northern Hemisphere snow cover, and excludes the influence of inter-annual variability of snow cover on snow phenology extraction, providing a novel perspective for identifying and understanding snow cover variations in the Northern Hemisphere.

How to cite: Wang, L., Miao, X., and Guo, W.: Dynamic identification of snow phenology in the Northern Hemisphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16791, https://doi.org/10.5194/egusphere-egu26-16791, 2026.

EGU26-17257 | ECS | Posters on site | HS2.1.4

Integrating snow-water equivalent simulated by a physically based model into a lumped model in an Alpine catchment in Italy 

John Mohd Wani, Giacomo Bertoldi, Michele Bozzoli, Daniele Andreis, and Riccardo Rigon

In the European Alps, seasonal snow plays a crucial role in hydrology, functioning as a reservoir by storing precipitation during winter and releasing it during the summer. Snow is highly sensitive to climate change, particularly in low- and mid-elevation mountain regions like the European Alps. In snow-fed basins, any changes in snowmelt contribution to river discharge can significantly impact agriculture, domestic water supply, and hydro power generation. 

Hydrological modeling employs a variety of models, ranging from simple lumped models to physically-based, spatially distributed models, to simulate river discharge. These models either have a simple temperature-based or a physically based snow module to simulate the snow dynamics. Distributed, physically based models can provide accurate insights into snow dynamics. However, their high input data requirement, over-parameterization, and high computational demands make them challenging to calibrate for discharge estimation for operational purposes. In contrast, simple lumped models require less input data, standard snow parameters, quick calibration, and are well-suited for operational applications, but, of course, lack spatial details.

In this study, we present an approach to improve both runoff forecasting and spatial snow pattern estimation by integrating the snow water equivalent (SWE) simulations from a physically based GEOtop model into the lumped GEOframe system. We utilize a mass-conserving Topographic Response Unit (TRU) aggregation logic to preserve the spatial variability of melt fluxes across elevation and aspect gradients. The methodology is applied in the Non Valley catchment, Italy, where water is important for agriculture, hydropower, and other uses.

Our results for the period 01-01-2017 to 15-09-2022 at hourly time step show that the GEOframe is able to simulate the discharge very well with a Kling-Gupta Efficiency (KGE) value of 0.87 and 0.72 during the calibration and validation, respectively. Substituting the internal snow module with GEOtop-derived fluxes yielded a KGE of 0.71 without further calibration. This demonstrates that the physically-based snow input successfully maintains the model’s predictive power while providing a more realistic and spatially distributed representation of snow dynamics. This coupling approach preserves the operational efficiency of lumped models while incorporating the improved physical representation and spatial variability essential for modeling mountain hydrology under a changing climate.

Acknowledgement

JMW and RR would like to thank and acknowledge the funding support from Project “SPACE IT UP! ASI Contract n.2024-5-E.0 CUP Master n. I53D24000060005” SAP fund n: 000040104905.

How to cite: Wani, J. M., Bertoldi, G., Bozzoli, M., Andreis, D., and Rigon, R.: Integrating snow-water equivalent simulated by a physically based model into a lumped model in an Alpine catchment in Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17257, https://doi.org/10.5194/egusphere-egu26-17257, 2026.

EGU26-17888 | ECS | Orals | HS2.1.4

SNOWCOP: Advancing High-Resolution Retrospective SWE Reconstruction in the Andes of Chile and Argentina with Remote Sensing 

Valentina Premier, Diego Blanch, Paloma Valentina Palma, Maria Ignacia Orell, Ezequiel Toum, Mariano Masiokas, Pierre Pitte, Leandro Cara, James McPhee, and Carlo Marin

SNOWCOP is a Horizon Europe project aimed at developing and evaluating a new high-resolution reanalysis dataset of snow water equivalent (SWE) and glacier ice melt rates for the extra-tropical Andes. The project integrates Copernicus and complementary remote sensing products within a physically based modeling framework to generate daily SWE and ice melt rate maps at 50 m spatial resolution, covering the period from 2002 to the present. These products address a critical observational gap in the region, where ground-based snow and meteorological measurements remain sparse. To support the development and validation of the SNOWCOP workflow, the initial phase of the project focuses on two pilot basins: the Río Maipo (Chile) and the Upper Río Mendoza (Argentina). These basins were selected due to their long term and high-quality instrumental SWE records, making good candidates for method’s evaluation.

We present the first results of a retrospective SWE reconstruction that integrates high-resolution daily snow cover maps with snowmelt modeling. The snow cover products are generated by applying a gap-filling and downscaling algorithm to coarse-resolution snow cover fraction data fused with high-resolution multi-source optical observations (Premier et al., 2021). Several snowmelt modeling approaches are evaluated, including a simple temperature-index (TI) model, an enhanced temperature-index (ETI) model (Pellicciotti et al., 2005), and fully physics-based formulations. Model coefficients are derived through calibration against in-situ observations. Meteorological forcings are obtained from ERA5 reanalysis data and dynamically downscaled using MicroMet (Liston & Elder, 2006). The reconstructed SWE is evaluated against ground-based measurements and compared with an existing SWE reanalysis dataset (Cortés & Margulis, 2017). as well as  modeling results produced by our team (CHM model - Marsh et al., 2020). 

 

References 

Cortés, G., & Margulis, S. (2017). Impacts of El Niño and La Niña on interannual snow accumulation in the Andes: Results from a highresolution 31 year reanalysis. Geophysical Research Letters, 44(13), 6859-6867. 

Liston, G. E., & Elder, K. (2006). A meteorological distribution system for high-resolution terrestrial modeling (MicroMet). Journal of Hydrometeorology, 7(2), 217-234. 

Marsh, C. B., Pomeroy, J. W., and Wheater, H. S.: The Canadian Hydrological Model (CHM) v1.0: a multi-scale, multi-extent, variable-complexity hydrological model – design and overview, Geosci. Model Dev., 13, 225–247. 

Pellicciotti, F., Brock, B., Strasser, U., Burlando, P., Funk, M., & Corripio, J. (2005). An enhanced temperature-index glacier melt model including the shortwave radiation balance: development and testing for Haut Glacier d’Arolla, Switzerland. Journal of glaciology51(175), 573-587. 

Premier, V., Marin, C., Steger, S., Notarnicola, C., & Bruzzone, L. (2021). A novel approach based on a hierarchical multiresolution analysis of optical time series to reconstruct the daily high-resolution snow cover area. IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, 14, 9223-9240. 

How to cite: Premier, V., Blanch, D., Palma, P. V., Orell, M. I., Toum, E., Masiokas, M., Pitte, P., Cara, L., McPhee, J., and Marin, C.: SNOWCOP: Advancing High-Resolution Retrospective SWE Reconstruction in the Andes of Chile and Argentina with Remote Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17888, https://doi.org/10.5194/egusphere-egu26-17888, 2026.

EGU26-17903 | Posters on site | HS2.1.4

Understanding the combined impact of vegetation and glacier change on Andean hydrology 

Catriona L. Fyffe, Katy Medina, Rolando Cruz, Edwin Loarte, Joshua Castro, Thomas E. Shaw, Simone Fatichi, Harol Granados, and Francesca Pellicciotti

The Peruvian Andes have faced substantial glacier loss in recent decades, and as the glaciers have receded, the exposed ground has been gradually occupied by succession vegetation. Previous work assessing the impact of glacier loss on downstream hydrology has tended to assess the cryospheric change in isolation, which may not account for the impact of vegetation changes on the water balance, especially in terms of altering catchment losses. An increasing body of work has demonstrated the importance of snow and glaciers for water resources in this region, especially in the dry season, although continued warming and glacier loss is predicted to decrease these meltwater contributions. Plant growth in deglaciated regions has the potential to compound runoff decreases through increasing evapotranspiration, but few studies have attempted to quantify this. This work aims to provide the first integrated assessment of the combined impact of glacier evolution and post-glacial vegetation succession on water availability in the Peruvian Andes. 

Here we quantify these changes by modelling the hydrological and ecological functioning of the Shallap catchment (13.6 km2) in the Rio Santa basin of the Peruvian Andes. We apply the mechanistic land surface model Tethys-Chloris which applies a full energy balance approach to resolving the fluxes over clean and debris-covered ice, snow and vegetation surfaces. The model is applied for a present period (2014-2025), forced by measured meteorological data, and using data from vegetation transects to parameterise the succession vegetation cover. The model is validated against ablation stakes, remotely sensed glacier mass balance, ground temperature, soil moisture and river discharge. We then simulate scenarios of climate, vegetation and glacier change to assess the separate and combined impact of glacier change and plant succession on the energy and water balance into the future. We are able to determine the impact of succession vegetation on evapotranspiration rates and water yield compared to bare soil and glacier cover, and determine the overall potential impact of glacier and vegetation change on downstream runoff. This work will provide a basis for understanding the significance of plant succession for the overall water balance in deglaciating catchments, impacting strategies for larger scale catchment and water management modelling throughout the Andes. 

How to cite: Fyffe, C. L., Medina, K., Cruz, R., Loarte, E., Castro, J., Shaw, T. E., Fatichi, S., Granados, H., and Pellicciotti, F.: Understanding the combined impact of vegetation and glacier change on Andean hydrology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17903, https://doi.org/10.5194/egusphere-egu26-17903, 2026.

EGU26-18389 | ECS | Orals | HS2.1.4

Impact of Snow Data Assimilation on Land-Surface Energy Fluxes at Sites Across Europe Using eCLM-PDAF 

Buliao Guan, Lukas Strebel, Johannes Keller, Harrie-Jan Hendricks Franssen, Gabrielle De Lannoy, and Bibi S. Naz

Snow plays a key role in land-surface processes by modulating the surface energy balance, soil thermal insulation and water availability. However, the influence of snow on water and energy fluxes in land surface models remains insufficiently understood. To improve simulations of the coupled water–energy cycle, we developed a snow data assimilation (snow-DA) within the Encore Community Land Model coupled to the Parallel Data Assimilation Framework (eCLM-PDAF; https://github.com/HPSCTerrSys/eCLM), enabling assimilation of both snow depth and snow water equivalent (SWE). In the Snow-DA experiment, we assimilate daily snow depth with a one-dimensional Ensemble Kalman Filter (EnKF), updating the liquid and ice SWE components across all snow layers; snow depth is then adjusted through its correlation with SWE. We evaluated the performance of the snow-DA framework by comparing snowpack variables as well as heat fluxes such as latent heat flux (LE), sensible heat flux (SH), ground heat flux (GH), and soil temperature, between data assimilation (DA) and open-loop (OL) simulations at eleven selected Integrated Carbon Observation System (ICOS) sites across Europe. The sites span different observation periods within 2017–2024. Each OL and DA experiment used 100 ensemble members, generated through perturbation of meteorological variables and key snow related parameters.  A multiplicative inflation factor of 0.95 and observation error of 0.2m are applied across all sites. Results across ICOS sites showed that DA substantially improved snow variable estimates compared to OL simulations. On average, the root mean square error (RMSE) of SD decreased by 27.3%, and the correlation coefficient (R) increased by 0.06. DA also improved the timing of snow cover duration, yielding a more realistic seasonal snow cover evolution when compared with satellite-based observations. Although overall changes in land-surface heat fluxes were modest, the improved snowpack reduced RMSE during the melt season for LE by 9.5%, evaporative fraction (EF) by 1.6%, and soil temperature by 20.8%. Although the energy balance was evaluated, and LE and EF improved, snow DA degraded the performance of SH and GH at most sites, indicating possible coupling bias between modeled variables for energy partitioning, or representativeness errors between tower-based and modeled fluxes. Overall, this study enhances the representation of snow processes in a land surface model and encourages further research into the modeling of associated water and energy balance mechanisms. Future work will investigate regional responses of water flux components, including runoff, evapotranspiration, and soil water content, to further examine snow data assimilation impacts on water availability.

How to cite: Guan, B., Strebel, L., Keller, J., Hendricks Franssen, H.-J., De Lannoy, G., and S. Naz, B.: Impact of Snow Data Assimilation on Land-Surface Energy Fluxes at Sites Across Europe Using eCLM-PDAF, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18389, https://doi.org/10.5194/egusphere-egu26-18389, 2026.

EGU26-18889 | Posters on site | HS2.1.4

Past and Future Evolution of the Gébroulaz Glacier. Modelling the impact on the Hydrology of the Doron des Allues in the Vanoise Massif 

Matthieu Le Lay, Adrien Gilbert, Kevin Pinte, Charlotte Jouet, Olivier Laarman, and Delphine Six

The Alps, often referred to as Europe's water tower, are undergoing profound changes as a result of climate change. Declining snow cover, accelerated glacier retreat, and increasingly severe periods of low flow raise urgent questions for water resource management, biodiversity, and energy security. Hydropower, one of the pillars of the European renewable energy strategy, is particularly exposed to these changes. To understand and anticipate these impacts, it is necessary to have detailed modeling of Alpine hydrological systems, combined with reliable climate projections.

To meet these challenges, the spatially distributed hydrological model MORDOR-TS (Garavaglia et al., 2017; Rouhier et al., 2017) now includes an explicit glacier component to simulate glacier dynamics in warming scenarios (Rouzies et al., 2024). Applied to the Isère basin in the French Alps, this model supports strategic decisions relating to hydroelectric exploitation by simulating hydrological responses at the basin scale under different future climate scenarios (Le Lay et al., 2022). However, glaciers remain relatively poorly instrumented today, and their ice volumes are often poorly known, making such modeling inevitably imprecise. In this context, local observations and modeling produced by glaciologists are valuable for better quantifying the relative contribution of glaciers to river flows and improving the robustness of hydrological projections.

This study focuses on the modeling of a representative alpine glacier in the Vanoise massif, which feeds the Doron des Allues River. On this glacier, combining historical glaciological monitoring with radar-based surveys of current geometry and ice volume has enabled a detailed modelling of the glacier geometry, its evolution and meltwater discharge throughout the 21st century. These data are used to refine glacier representation in the MORDOR-TS hydrological model —surface area, volume, and meltwater flows—improving the reliability of basin-scale hydrological simulations, distinguishing between precipitation-driven and glacier-driven contributions. Results confirm strong consistency between the local glaciological model and the regional hydrological model and highlight pathways for further parameterization improvements.

The glacier is projected to almost completely disappear by 2100, with cascading impacts on discharge regimes. Beyond reduced mean flows, significant shifts in seasonal patterns and diminished summer flows are expected—posing challenges for hydropower production, ecosystem resilience, and water allocation. These results highlight the importance of coupling regional  hydrological models with high-resolution glaciological data to improve the robustness of climate impact assessments in mountain regions.

These findings underscore the urgency of adaptation strategies for mountain water resources in a warming climate. They also illustrate the value of coupling large-scale hydrological models with high-resolution glaciological data to support energy planning and climate resilience across Europe’s alpine regions.

How to cite: Le Lay, M., Gilbert, A., Pinte, K., Jouet, C., Laarman, O., and Six, D.: Past and Future Evolution of the Gébroulaz Glacier. Modelling the impact on the Hydrology of the Doron des Allues in the Vanoise Massif, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18889, https://doi.org/10.5194/egusphere-egu26-18889, 2026.

EGU26-19296 | ECS | Orals | HS2.1.4

Flash Snow Drought: Escalating Risks to Mountain Water Resources at local scale 

Hemant Singh, Md Mehraj, and Divyesh Varade

Snow plays a critical role in water resources, the planetary energy balance, glacier nourishment, ecosystem and the winter tourism economy. In recent decades, rising temperatures have led to a decline in snowfall and shifting of patterns. These changes have resulted in reduced snowpack and earlier snowmelt, thereby triggering snow drought conditions. Since the first formal definition of snow drought in 2017, the topic has gained increasing scientific attention, with the first systematic studies published in 2019, followed by significant advancements in subsequent years. However, flash snow droughts (FsD) have not yet been studied and remain unexamined. FsD are short-duration events characterized by rapid onset and intensification, occurring over timescales ranging from weeks to month. These events may arise due to low precipitation accompanied by warm winter. Consequently, establishing a clear definition and identifying FsD hotspots are critical, particularly in regions experiencing imbalanced seasonal snow patterns and low snowpack. In this work, we examine FsD at a 500 m spatial resolution in the North-West Basin part of Afghanistan of the Hindu Kush Himalaya (HKH) using a Snow Water Equivalent Index (SWEI) derived from the High Mountain Asia Snow Reanalysis (HMASR) dataset. The analysis is limited to the 1999–2016 water years due to the unavailability of HMASR data for more recent periods. It is also noted that coarser-resolution datasets may be inadequate for capturing FsD events because of spatial heterogeneity in snow cover dynamics. Our results indicate the recurrence of flash snow droughts (FsDs) with varying durations, notably during February-March 2001, November-December 2010, and January 2011 and 2014. These FsDs fall within the moderate to severe drought categories, based on a threshold of −1. This study highlights the importance of FsD at the local scale for policymaking, mitigation planning, and integrated monitoring frameworks, and it identifies key research gaps to support resilient FsD management.

How to cite: Singh, H., Mehraj, M., and Varade, D.: Flash Snow Drought: Escalating Risks to Mountain Water Resources at local scale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19296, https://doi.org/10.5194/egusphere-egu26-19296, 2026.

EGU26-19867 | Posters on site | HS2.1.4

Glacio-hydrological modeling informed by observations from a research basin in the Central Andes of Chile 

James McPhee, Noemi Villagra, Pablo Mendoza, and María Courard

Water resources availability in the Central Andes of Chile largely depends on glacier melt, which is undergoing accelerated changes as a consequence of global warming. Studying the hydrological response of glacierized systems requires understanding their interaction with catchment-scale processes, which in turn demands detailed observations that are rarely available in glacierized basins. Physically based hydrological modeling offers the opportunity of representing processes at large spatial extents through the informed selection and transference of observable parameters. Here, the Cold Regions Hydrological Model (CRHM) was implemented to evaluate the feasibility of transferring parameters from the intensively monitored Glaciar Echaurren Research Basin (app. 4 km2) to two larger glacierized basins: the Yeso River basin at Termas del Plomo (RYTP, app. 60 km2) and the Mapocho River basin at los Almendros (RMLA, app. 640 km2).

Simulations were performed using both locally calibrated parameters and parameters transferred from the experimental basin, and model performance was evaluated in terms of streamflow, fractional snow-covered area (fSCA), and snow water equivalent (SWE). Full transfer of the calibrated parameters from the small intensive study catchment to the larger RMLA basin resulted in reductions of up to 71% in streamflow KGE and 97% in SWE NSE compared to the basin’s own calibration. In the intermediate RYTP basin, the transfer of snow-related parameters adequately reproduced the seasonal pattern of SWE, although with a −59.2% bias and a 70.6% decrease in streamflow KGE relative to the calibrated version.

Individual parameter transfer revealed that snow-related parameters, such as snow roughness length and active layer thickness, explain a large fraction of the loss in SWE performance. On the other hand, the degradation in streamflow performance was dominated by parameters associated with surface storage processes. Overall, the results indicate that parameter transferability is only partially viable: while some parameters can be generalized across basins with similar characteristics, highly sensitive and locally dependent parameters require site-specific calibration to preserve model representativeness.

How to cite: McPhee, J., Villagra, N., Mendoza, P., and Courard, M.: Glacio-hydrological modeling informed by observations from a research basin in the Central Andes of Chile, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19867, https://doi.org/10.5194/egusphere-egu26-19867, 2026.

EGU26-19982 | Orals | HS2.1.4

How Much Climate Information Does a (Temperature Index) Snow Model Need? 

Ross Woods, Adria Fontrodona-Bach, Josh Larsen, and Bettina Schaefli

Changes in snowpack climatology are taking place because of changes in climate. Information is needed on how future changes in climate may affect snowpack regimes.

This information is usually generated by running time stepping models for which time series of forcing data must be supplied. In this study we explore whether it is possible to make reliable estimates of snowpack regime without explicit knowledge of the temporal sequence of forcing data. This could support development of a hydrological theory of seasonal snowpacks. We will test whether it could be enough to know some statistics of the forcing data, rather than the complete time series. In this presentation, we begin by trying to identify where it is necessary to maintain the correlation between temperature and precipitation amount in a temperature index model. Our interest is in correlations at the timescale of a precipitation event; seasonal-scale correlations will be captured separately.

We investigate these questions at 4736 locations in the northern hemisphere, using the NH-SWE database combined with precipitation (P) and temperature (T) data from GHCN. We run the temperature index model once with the original forcing data, and then again with the temperature data displaced by a few days in time from the precipitation data, to reduce their cross-correlation. We calculate statistics of the modelled snowpack for the two model runs (for each station and each year: the start date, peak date and end date for the snowpack, and the peak SWE – snow water equivalent). If the cross-correlation is not important, then the statistics of modelled snowpack should not change much between the two model runs. Since our interest is in snow accumulation and melt, we expect that the most important P-T correlations are at times of year when both rainfall and snowfall are likely to occur.

Initial results show that for the 60% of sites with a positive correlation between P and T-anomaly, neglecting the correlation generally leads to an overestimation of peak SWE (by an average 12%). The overestimation presumably occurs because when the correlation is removed, days below freezing are more likely to be paired with the higher precipitation amounts which tend to occur on days above freezing, and thus the amount of snowfall is increased by neglecting the correlation.   For the remaining sites with a negative correlation between P and T-anomaly, neglecting the negative correlation generally leads to a slight underestimation of peak SWE (by an average -4%).

We will also carry out several other similar model experiments with degraded forcing to identify key features of the climate data. The intended endpoint of the work is an improved theory of snowpack hydrology, i.e., a stochastic version of the deterministic theory in Woods 2009 (https://doi.org/10.1016/j.advwatres.2009.06.011)

How to cite: Woods, R., Fontrodona-Bach, A., Larsen, J., and Schaefli, B.: How Much Climate Information Does a (Temperature Index) Snow Model Need?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19982, https://doi.org/10.5194/egusphere-egu26-19982, 2026.

EGU26-20199 | Posters on site | HS2.1.4

Aufeis (Proglacial Icing) in the forefield of a land-terminating outlet glacier in West Greenland – multi-annual and seasonal variability and drivers  

Jakob Abermann, Andreas Truegler, Harald Zandler, Helena Bergstedt, Florina Schalamon, Sebastian Scher, and Wolfgang Schöner

In this contribution, we share observations of a braided river plain adjacent to the little ice age moraine of a land-terminating outlet glacier in West Greenland at around 71°N. During three visits in spring (2023 - 2025), we document a plain of refrozen water. We report on the extent, genesis and decay of the aufeis plain and hypothesize on drivers building it. Time-lapse and high-resolution satellite imagery allow us to assign the build-up of the aufeis during core winter until spring and the decay throughout the melting season. We find that long after the disappearance of the snow cover at the adjacent glacier and ice-free environment, the aufeis still is in place. Using multispectral satellite imagery (Sentinel-2) we derive a time series of aufeis extent ranging from virtually no coverage to almost 0.5 km² for the period 2016-2025, using a random forest classification. DEM differences derived from photogrammetric acquisitions using UAVs enable us to estimate ice volumes between 49x10³ (April 2025) and 110x10³ m³ (April 2024), respectively. To understand atmospheric conditions for meltwater generation, we use automated weather station data near the aufeis plain. As another reason for ice formation, we discuss potential water sources related to groundwater aquifers in porous ground moraine material. Finally, bias-corrected CARRA model output was applied to reconstruct meteorological conditions relevant for aufeis formation. Based on a lagged correlation approach, we find statistically significant (p = 0.05) correlations between cumulative positive air temperature departures and aufeis extent summing up approx. 7 years before the respective icing occurrence. While simplified, we discuss a possible long-term relation between icing extent and meltwater generation.

How to cite: Abermann, J., Truegler, A., Zandler, H., Bergstedt, H., Schalamon, F., Scher, S., and Schöner, W.: Aufeis (Proglacial Icing) in the forefield of a land-terminating outlet glacier in West Greenland – multi-annual and seasonal variability and drivers , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20199, https://doi.org/10.5194/egusphere-egu26-20199, 2026.

EGU26-20774 | ECS | Orals | HS2.1.4

Modelling Seasonal and Decadal Variability of Snow Conditions across Finland using SnowModel  

Ashutosh Taral, Ioanna Merkouriadi, Anna Kontu, Kati Anttila, and Pertti Ala-Aho

Snow, including both seasonal and perennial snow cover plays an important role in regulating surface energy balance, water availability, and hydrological processes in high-latitude and mountainous regions. Finland, located in the boreal and subarctic zone, experiences long winters with extensive snow cover and exhibits substantial spatial and temporal variability in snow accumulation, structure, and melt dynamics. While Finland has extensive in situ snow observations, a nationally consistent, high-resolution (e.g., 250 m), multi-decadal reconstruction of snow water equivalent (SWE), snow depth, and snow density that integrates distributed physical modelling with observational data assimilation is still lacking. Understanding how these snow processes evolve seasonally and over decadal timescales is essential for assessing climate change impacts on Nordic cryosphere–hydrology systems and for improving predictive capabilities at regional to national scales.

This study uses SnowModel (Liston & Elder, 2006), a physically-based, distributed snow evolution model, to simulate snowpack processes across Finland over the past three decades (1990-2024). The model runs at a 3-hourly internal time step, with analysis conducted at a daily temporal scale at 250 m spatial resolution. The meteorological forcing is derived from a high-resolution (10 km) NORA10 reanalysis dataset, ensuring consistent spatial coverage for the study domain. The static surface inputs includes a 10 m digital elevation model from the National Land Survey of Finland and CORINE land cover data from Finnish Environment Institute ( SYKE; 25 m), resampled to the model grid enabling a detailed representation of snow processes across diverse Finnish landscapes.

The modelling framework in our study explicitly focuses key on snow variables, including snow depth, snow density, snow water equivalent (SWE), snowmelt timing, and snowmelt runoff. To improve realism and robustness, the simulations incorporate data assimilation of long-term in situ snow observations, primarily snow depth and SWE, from a nationwide network of stations. Model evaluation is conducted using independent observational datasets helping SnowModel accurately capture Finland’s spatial and temporal snow variability.

The analysis is designed to characterise both seasonal snow dynamics and long-term snow variability across Finland. Seasonal behaviour is examined through time series analysis and interannual variability of snow accumulation and melt, while long-term changes are assessed using spatial trend analyses and decadal comparisons. Emphasis is placed on contrasting snow regimes across southern, western, eastern, and northern Finland, reflecting the influence of maritime effects from the Baltic Sea, continental climate in eastern regions, and persistently cold conditions in northern Lapland.

By combining the high-resolution modelling with extensive snow observation datasets, our study aims to establish a multi-decadal snow reconstruction using a physically distributed model and provide a national-scale baseline of snowpack variability under changing climate conditions. The results are expected to provide valuable insights into evolving snow processes in boreal and sub-Arctic environments, supporting hydrological and climate impact studies, and contribute to improved cryospheric modelling frameworks for northern Europe.

How to cite: Taral, A., Merkouriadi, I., Kontu, A., Anttila, K., and Ala-Aho, P.: Modelling Seasonal and Decadal Variability of Snow Conditions across Finland using SnowModel , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20774, https://doi.org/10.5194/egusphere-egu26-20774, 2026.

The Tibetan Plateau (TP), often referred to as the “Asian Water Tower,” hosts extensive cryospheric resources that are highly sensitive to climate warming. The Qilian Mountains (QL), located in the northeastern TP, constitute a key ecological security barrier in western China and a strategic corridor of the Silk Road Economic Belt. Based on multi-source datasets and the runoff coefficient method, we estimate the mean annual runoff of the Qilian Mountains to be approximately 15.671 billion m³. River basins originating in the eastern Qilian Mountains exhibit a clear declining trend in annual runoff, whereas most basins in the central and western regions show increasing trends, suggesting that sustainable water resource development in the eastern Qilian Mountains faces greater challenges under continued warming.

Thus, we chose the Beichuan River Basin which is located in the eastern Qilian Mountains as the study area. A snowmelt pathway-tracking algorithm and a reservoir operation scheme were integrated into a high-resolution, physically based distributed hydrological model (DHSVM) to investigate the mechanisms of runoff generation. The results indicate that both the annual snow contribution to soil moisture (SC-SM) and the snow contribution to streamflow (SC-S) declined significantly from 1965 to 2019. At the monthly scale, SC-SM exhibited the largest amplitudes in the upper soil layer, while peak contributions in deeper layers lagged behind those of the shallow layer. In addition, mean monthly SC-S across all stations displayed a distinct bimodal pattern associated with the seasonal snowfall regime. Reservoir regulation measures only exerted minimal impacts (≤2.0 %) on SC-S. Furthermore, based on long-term meteorological observations, we analyzed the spatiotemporal variability of the temperature lapse rate and its associated hydrological responses.

How to cite: Liu, Z.: Hydrological responses to climate warming for mountainous regions in the northeastern Tibetan Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21457, https://doi.org/10.5194/egusphere-egu26-21457, 2026.

EGU26-21723 | ECS | Posters on site | HS2.1.4

Multidecadal snow water equivalent reconstruction in Central Italy using the Multiple Snow Data Assimilation System 

Mohsin Tariq, Esteban Alonso-González, Manuela Girotto, Francesco Avanzi, Mauro Rossi, Paolo Stocchi, Paolo Tuccella, and Christian Massari

Reliable estimates of snow water equivalent (SWE) are necessary to understand hydrological variability and snow-related extremes in mountain environments of Central Italy and the Apennines, where snowpacks are generally thin, variable, and still insufficiently observed by conventional monitoring networks. As part of broader efforts to improve how snow processes are represented in complex terrain, this work describes the recent developments using the Multiple Snow Data Assimilation System (MuSA). The primary goal of this work is to generate spatially coherent SWE estimates over Central Italy.

The modelling approach employs a physically based snow model within MuSA, driven by MORE meteorological reanalysis (MOloch-downscaled ERA5 REanalysis), which provides high-resolution atmospheric forcing at ~1.8 km over Italy spanning more than three decades from 1990 onward, enabling consistent multidecadal SWE reconstruction. This extended forcing, available at an hourly scale and with a finer spatial resolution, captures the complex orographic precipitation and temperature gradients that are critical for accurate snowpack simulation in the Apennines.  Snow depth observations from Sentinel-1 (S-1) are assimilated as the primary observational input, leveraging their spatial extent and ability to detect snowpack characteristics in areas with limited ground measurements. Given that S-1 snow depth is only available from around 2015 onward, the main objective of this research is to use an observation-constrained MuSA configuration to extrapolate the SWE estimate back to 1990, producing multidecadal records.

The methodological design, data preparation, and assimilation strategy are described to ensure temporal consistency between the observation-rich and pre-observation period. Specific focus is given to basin-scale implementation, uncertainty estimation, and potential scalability to regional-scale applications. Presently, model validation and analysis of SWE are ongoing. This research establishes a concrete framework for long-term SWE estimation in Central Italy. It provides future studies with the opportunity to assess snow variability and extremes at the regional scale in a changing climate.

How to cite: Tariq, M., Alonso-González, E., Girotto, M., Avanzi, F., Rossi, M., Stocchi, P., Tuccella, P., and Massari, C.: Multidecadal snow water equivalent reconstruction in Central Italy using the Multiple Snow Data Assimilation System, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21723, https://doi.org/10.5194/egusphere-egu26-21723, 2026.

The proportion of annual precipitation that falls as snow, called snow fraction (Sf), in the western United States is declining. The impact of this transition on streamflow timing and magnitude is unclear.  Some studies report declining runoff efficiency (streamflow/precipitation, RE) with declining Sf , while others report no change and even increases. The causes of variability in the Sf-RErelationship involve complex interactions between climate and landscape properties. To understand and perhaps mitigate the impact of declining Sf on water resources, it is essential to be able to represent the physical processes and properties controlling that variability in predictive models. While significant insights in SfRErelationships across catchments have been revealed in recent years, few have investigated the variability within a catchment over time. Here, we report Sf-RE relationships from two long-term, highly instrumented catchments in the rain-to-snow transition zone in southwest Idaho, USA. The Dry Creek Experimental Watershed (DCEW) and the Reynolds Creek Experimental Watershed (RCEW) have been monitoring hydrometeorological variables for approximately 25 and 60 years, respectively. Analyzing these long-term records allows us to identify potential physical mechanisms controlling the Sf-RE relationship that short-term, spatially-focused studies cannot. Preliminary results suggest that variability in the alignment of energy and water availability across the rain-dominated to snow-dominated elevation gradient controls how snow fraction impacts streamflow response.

How to cite: McNamara, J.: Impact of decling snow fraction on runoff efficiency in the rain-snow transition zone., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21980, https://doi.org/10.5194/egusphere-egu26-21980, 2026.

EGU26-22177 | Orals | HS2.1.4

Advancing Snow Observation Systems to Improve Hydrologic Prediction in Mountain Headwaters 

S. McKenzie Skiles, William Roe, and Steven Clark

Snow energy balance, particularly radiation balance, is monitored only at a limited number of well-instrumented, research-focused snow study sites in the western United States. This lack of observations limits our ability to force or validate process-based snow models in mountain terrain, an important hurdle to operational adoption. To address this gap, we have prototyped a low-cost, low-power, transportable snow monitoring system capable of transmitting near-real-time snow energy balance relevant observations. Each instrumentation suite measures incoming and reflected broadband shortwave radiation, incoming and emitted longwave radiation, air temperature/relative humidity, and snow depth. Including sensors, power, data logging, and communications infrastructure, each site costs less than USD $10,000, enabling deployment at a scale not feasible with conventional research stations. The systems have been deployed at 11 sites across snow-dominated headwater catchments in the Intermountain West, more than doubling the current number of snow radiation balance observation sites. Two sites are co-located with research sites for validation, and observations are used to drive the 1d SNOBAL model to assess the sensitivity of simulated snow water equivalent to lower-cost instrumentation. This approach complements existing snow monitoring networks, including the ~900-site SNOTEL (Snowpack Telemetry) network, which provides long-term observations for snow mass balance monitoring and index-based streamflow forecasting. SNOTEL sites are intentionally located in sheltered, mid-elevation forest openings and do not capture spatial variability, nor do they measure radiation balance. Low-cost, distributed energy balance observations provide a pathway to complement and extend the observational capabilities of current networks.

How to cite: Skiles, S. M., Roe, W., and Clark, S.: Advancing Snow Observation Systems to Improve Hydrologic Prediction in Mountain Headwaters, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22177, https://doi.org/10.5194/egusphere-egu26-22177, 2026.

EGU26-23257 | ECS | Posters on site | HS2.1.4

Investigating Snow and Firn Processes in a Georgian Glacier through Local Data and Modeling 

Sopio Beridze and Carlo De Michele

Mountain glaciers in data-scarce regions are particularly sensitive to climate variability, yet their snow and
firn processes remain poorly constrained due to limited long-term observations/analyzes, especially in the
Caucasus region. Caucasus glaciers are highly sensitive to temperature and precipitation variability due to
their mid-latitude location, steep relief, and strong seasonal contrasts.
In this study, we present a preliminary analysis of snow accumulation and melt dynamics for selected
areas in Georgia (Racha Region, Buba glacier), based on in situ meteorological observations and historical
data. The analysis focuses on preparing meteorological input data for the application of a conceptual
snow–firn model, following the framework proposed by Banfi and De Michele (2021). Meteorological and
snow data from selected Georgian glacierized catchments are analyzed to characterize snow
accumulation and melt dynamics and to prepare input datasets for snow–firn modelling. Particular
attention is given to precipitation phase partitioning, seasonal snow persistence, and data harmonization,
as available observations are often heterogeneous and affected by temporal gaps.
Key variables include snow depth, snow bulk density, snow water equivalent (SWE), and meltwater runoff.
While such variables are monitored at several well-instrumented Alpine sites, allowing for extensive multi-
year model evaluation, comparable long-term and structured datasets remain scarce in the Caucasus
region. However, given the similarities between the Caucasus region and the Italian Alps in terms of
geomorphological and hydrological characteristics, the modelling framework is well suited for application
in the Caucasus context.

How to cite: Beridze, S. and De Michele, C.: Investigating Snow and Firn Processes in a Georgian Glacier through Local Data and Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23257, https://doi.org/10.5194/egusphere-egu26-23257, 2026.

Landslides are among the most destructive natural hazards in Türkiye, where high susceptibility is linked to active tectonic structures, steep topography, and complex climatic conditions. For instance, the Eastern Anatolian Region is recognized as a high-risk zone regarding seismicity and vast mass movements; therefore, reliable predictive tools for hazard mitigation are needed. Although several studies have already applied Machine Learning (ML) methodology for Landslide Susceptibility Mapping (LSM) problems in Türkiye, no systematic comparative evaluation of different modelling hierarchies has been performed so far for this particular area in a tectonically complex environment.

This study attempts to fill this gap by developing and rigorously comparing three disparate modeling methods: a statistical baseline, Logistic Regression (LR); an ensemble, Random Forest (RF); and a state-of-the-art deep learning method, Convolutional Neural Networks (CNN). The study was conducted using a landslide inventory and twelve landslide conditioning factor layers, including topographic data: DEM, Slope, Curvature, TWI; geological data: Lithology and Distance to Fault; environmental data: NDVI and Land Cover.

The core methodology embraced a systematic optimization of dataset splitting, whereby model performance was compared across different test/train ratios in order to identify the most stable and accurate data partition. Results are presented using key statistical metrics, including Accuracy and the Area Under the Receiver Operating Characteristic Curve (AUC-ROC), for LR, RF, and CNN. The best-performing model and its corresponding optimal test/train ratio were used to generate the final high-resolution LSM map for the Muş-Bingöl area. This forms a scientifically validated tool that can be used for regional land-use planning and risk management.

How to cite: Erdoğan, N. and Akgün, H.: Landslide susceptibility mapping of the Muş-Bingöl region: a comparative analysis and optimization of machine learning models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-498, https://doi.org/10.5194/egusphere-egu26-498, 2026.

INTRODUCTION

Underground mining frequently leads to surface instability such as subsidence, sinkholes, and landslides. In the Bulqiza chrome mine in Albania, decades of extraction and the transition from cut-and-fill to sublevel stoping have increased rock-mass deformation, resulting in fissures, caving, and surface failures. This study focuses on Profile XIV, where both continuous subsidence and a sinkhole are present, in order to evaluate the accuracy of predictive methods used to assess mining-induced deformation.

AIM

This study aims to assess the surface impacts of underground mining in the Bulqiza district by applying both empirical subsidence modelling and numerical simulations using Finite Element Methods. The study compares predicted results with observed deformation, evaluates the influence of caved zones (goaf) and tectonic structures, and verifies the suitability of using a combined empirical and numerical approach for deformation assessment.

METHODS

Geological and mechanical properties were defined through field investigations and archived mine data. An empirical model with a subsidence coefficient of K = 0.9 was used to calculate the critical collapse depth (Hcal) and compare it with the effective mining depth (Hfac). Numerical simulations were then performed with the Rocscience FEM software for two surface-deformation profiles: one exhibiting continuous subsidence and the other featuring a surface sinkhole. Each profile was modelled under different conditions, including the presence or absence of goaf and the inclusion or exclusion of tectonic influence. Surface displacement was used as the main indicator for assessing deformation.

RESULTS

The empirical model indicated a low likelihood of funnel formation in the subsidence profile, where Hcal was smaller than Hfac, while in the sinkhole profile, Hcal exceeded Hfac, confirming a high probability of collapse consistent with field observations. Numerical modelling supported these findings. In the subsidence profile, vertical displacement remained small around 14 mm regardless of whether the goaf was included, and no funnel formation was predicted. In the sinkhole profile, displacement increased to 24.3 mm when the goaf was considered without tectonics. When tectonic effects were included, displacement increased substantially to values between 40.4 and 61 mm, closely reproducing the actual sinkhole conditions. These results show that tectonics strongly amplifies surface deformation.

CONCLUSIONS

This study demonstrates that both empirical and numerical methods effectively reproduce the types and magnitudes of surface deformation observed in the Bulqiza mine. Numerical modelling closely matched actual conditions, particularly when tectonic effects were incorporated. While goaf conditions had little effect in the subsidence zone, they significantly increased deformation in the sinkhole area. The findings confirm that tectonic structures are a major factor controlling surface collapse and that a combined empirical and numerical approach provides a reliable method for assessing mining-induced surface impacts in Bulqiza and comparable underground mining environments.

How to cite: Belba, P.: Surface Deformation Assessment in the Bulqiza Chrome Mine Using Empirical and Numerical Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-798, https://doi.org/10.5194/egusphere-egu26-798, 2026.

In recent years, extreme climate events characterized by heavy rainfall and seismic activity have significantly intensified the risks of slope disasters in Taiwan's mountainous regions. This study focuses on Zhongxing Village, Liugui District, Kaohsiung City, Taiwan, an area marked by steep topography and a recurrent history of severe landslides and debris flows. The primary objective is to evaluate slope stability under diverse environmental scenarios using numerical simulation. The methodology utilizes the STEDwin slope stability analysis software, specifically employing the Bishop method, which is based on limit equilibrium theory. A representative geographic profile near Shanping Villa was established, with soil parameters calibrated from 16 localized borehole records obtained from engineering geological databases. The analysis examines three critical conditions: normal, heavy rain, and earthquake. The findings indicate that under normal conditions, the factor of safety (FS) is 1.30, which falls short of the official standard threshold of 1.5 for permanent slope structures. Under the heavy rain scenario (with groundwater at the surface), the FS drops drastically to 0.66, representing a critical 49.23% reduction in stability. In the earthquake scenario, incorporating parameters from the 2016 Meinong earthquake, the FS reached 1.01. These results align closely with historical records from Typhoons Morakot and Kaemi, highlighting significant risks to Shanping Villa, Shanping Forest Road, and Highway 27. In conclusion, the drastic rise in the groundwater level is the primary driver of slope failure in this region. The study recommends the prioritized implementation of deep drainage systems, such as drainage galleries, to enhance soil effective stress. Furthermore, establishing a real-time monitoring and early warning system is essential to facilitate mandatory evacuations during extreme rainfall, thereby ensuring public safety and infrastructure resilience.

How to cite: Hsu, H.-H., Deng, X.-X., Chen, Y.-H., Chang, Y.-C., and Chen, Y.-H.: Slope Stability Analysis and Hazard Potential Assessment in Zhongxing Village, Kaohsiung City: Numerical Simulation under Extreme Rainfall and Earthquake Scenarios Using STEDwin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2417, https://doi.org/10.5194/egusphere-egu26-2417, 2026.

An increase in soil water content (SWC) from rainfall infiltration reduces the matric suction and shear strength; hence, rainfall is a primary trigger of shallow landslides. While accurate SWC monitoring is critical for predicting slope failure, traditional point-based sensors lack the spatial resolution required for effective field-scale assessment. This study aims to bridge this gap by integrating hyperspectral and multispectral imaging technologies with advanced machine learning (ML) models. Based on 114 in-situ soil samples collected from landslide-affected areas across South Korea, correlations between physical soil properties (e.g., void ratio, soil color) and hyperspectral data in the visible and near-infrared (Vis-NIR) regions were analyzed. Two ML algorithms, Random Forest (RF) and Multilayer Perceptron (MLP), were employed to develop predictive models for SWC. In this study, statistical evaluation indicated that the RF model demonstrated superior accuracy and robustness in handling high-dimensional spectral data compared to the MLP model. To validate the method's applicability for landslide monitoring, field tests were conducted in the mountainous region of Pyeongchang, South Korea, using a multispectral camera mounted on an unmanned aerial vehicle (UAV). The RF model successfully predicted the spatial distribution of SWC using spectral reflectance and geotechnical parameters. Although the model showed limitations in extrapolating beyond the training data range, it effectively captured critical variations in soil moisture relevant to slope stability. These results suggest that integrating UAV-based remote sensing with ML offers a promising, non-contact approach for high-resolution monitoring of shallow landslides, contributing to more proactive disaster prevention strategies.

How to cite: Lim, H.-H., Cheon, E., and Lee, S.-R.: UAV-Based Multispectral Assessment of Soil Water Content for Shallow Landslide Monitoring: A Machine Learning Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2879, https://doi.org/10.5194/egusphere-egu26-2879, 2026.

EGU26-2976 | ECS | Posters on site | NH3.3

Beyond Coarse Data: Soil Thickness and Rainfall forLandslide Hazard Modelling 

Paula Cortes, Johnny Vega, Robert Reinecke, and Ugur Ozturk

An increasing population in mountainous regions, where gentle and stable topography is scarce, drives residents to settle on steep slopes. These slopes are particularly prone to shallow landslides, which involve the displacement of the upper soil layers and are more easily triggered by rainfall. Therefore, accurate landslide hazard models are needed to safeguard populations.

These models typically include spatial data, such as soil thickness and rainfall. However, the lack of detailed inputs often means that models operate at coarse scales, which can mask local variability and potentially underestimate hazard levels. To address this gap, our research question is whether simulations of shallow landslides can be improved by enhancing the spatial resolution of two critical variables derived from coarse satellite data: (i) soil thickness determining the volume of material available for sliding, and (ii) rainfall controlling soil saturation and pore-water pressure dynamics.  

To demonstrate the scalability and applicability of the method to other regions prone to landslides, we tested this approach in La Estrella, Colombia, a municipality with a long history of landslides and rapid population growth on steep slopes. For soil thickness, we applied a geomorphological model that relates soil depth to slope angle and distance to the drainage network. We validated the estimates against borehole measurements, finding strong agreement at three of five test sites. For rainfall, we integrated CHIRPS with local rain-gauge data, using spatial interpolation and regression-based downscaling to produce high-resolution rainfall fields. The downscaling model was then evaluated using statistical metrics, including the Pearson correlation coefficient (r), bias, and Nash–Sutcliffe efficiency (NSE).

In the next step, we will feed these two outputs into a Landlab shallow landslide probability model that couples hydrological response with soil mechanical stability. This will allow us to quantify the influence of input resolution on predicted landslide probability patterns.

How to cite: Cortes, P., Vega, J., Reinecke, R., and Ozturk, U.: Beyond Coarse Data: Soil Thickness and Rainfall forLandslide Hazard Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2976, https://doi.org/10.5194/egusphere-egu26-2976, 2026.

EGU26-3757 | ECS | Orals | NH3.3

Environmental Controls on Post-Little Ice Age Landslide Distribution Around the South Patagonian Icefield 

Gernot Seier, Matěj Slíva, Tomáš Pánek, and Diego Winocur

Understanding landslide (LS) distribution in deglaciated mountains is key to landscape evolution and geohazard risk. We present an orogen-scale assessment of 1,691 Post-Little Ice Age (LIA) LSs (91% shallow) along the South Patagonian Icefield (SPI, 48–52°S) margins. Mapped via high-resolution multitemporal imagery (2010–2025) and multi-operator validated, kernel densities (10 km bandwidth) show clustering in western and southern SPI—central peak, northwest secondary—amid ~20% ice loss (since the end of the LIA) and uplift >40 mm/yr.

Environmental variables from LS/non-LS areas fed Bayesian horseshoe variable selection. Sparse Gaussian process regression (R2=0.96, SPAEF ≥0.85) identified precipitation, fault density, and uplift as dominant controls. Precipitation destabilizes slopes via pore pressures, triggering shallow LSs (positive correlation); fault density signals structural weakness/seismic facilitation; uplift shows complex negative LS correlation, as active deformation/steep slopes favor erosion over accumulation, reducing LS buildup. Lithology, permafrost, retreat rates exert weaker, context-dependent influences. LS versus non-LS distinctions underscore the value of integrating correlation-based and predictive approaches. Coupled climate-deglaciation-tectonics govern landslide distribution in the SPI.

Critically, ~17% of LSs overlap glacial lake upslope areas (30 m buffer), preconditioning glacier lake outburst flood risks at, e.g. Torre Glacier's ~8 Mm³ failure—shallow dominance may temper severity, sea-proximal cases extend threats. Findings illuminate paraglacial responses to glacier retreat, offering predictive hazard frameworks for warming cryosphere.

How to cite: Seier, G., Slíva, M., Pánek, T., and Winocur, D.: Environmental Controls on Post-Little Ice Age Landslide Distribution Around the South Patagonian Icefield, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3757, https://doi.org/10.5194/egusphere-egu26-3757, 2026.

Road construction on hillslopes has increased explosively due to the rapid socioeconomic development in China’s mountainous areas. The exposure of steep and rapidly weathering slopes caused by road construction accelerates slope movements, especially roads building on residual soil. Residual soil slopes are prone to slow movements and may evolve to failure in response to infiltration of rainwater. Engineering works on residual soil (e.g., excavation, filling for buildings and roads) exacerbate these problems through altering the internal and external stress of slopes. Yet our understanding of the interactive effects of rainfall and road construction on slope dynamics or even failure in subtropical residual soils remains elusive. Here, we used three-decadal radar remote sensing data to quantify the time series deformation before a catastrophic slope failure, occurring at Meida Highway in China that caused 52 fatalities. Physics-based decomposition of the time series movements over the past 8 years reveals that there is a constant seasonal movement related to rainfall and a precursory accelerated movement triggered by slope reinforced measures before failure occurrence in May 2024. Emergency mitigations of reinforced measures modified the infiltrates and routes of surface and subsurface water, leading to an adverse impact of reducing slope failure risk. Analysis of numerical simulation indicates that rainfall-induced pore water pressure reduced the shear strength of granite residual soils, ultimately triggering slope failure. This improved understanding of the slope dynamics in response to different forces will be important to avoid economic and life loss, strengthen emergency planning and identify potential risks.

How to cite: Huang, X. and Ma, P.: Satellite images reveal progressive slope deformation triggered by mountainous road construction in subtropical South China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4787, https://doi.org/10.5194/egusphere-egu26-4787, 2026.

EGU26-6955 | ECS | Orals | NH3.3

Cormons landslide characterization using Lidar and remote sensed data. 

alessia scalabrini, simone francesco fornasari, and giovanni costa

Landslides are a global phenomenon occurring in several climatic and geomorphologic contexts, generating billions in economic losses and causing thousand of causalities each year. This phenomenon is often characterized as a local problem, but its effect and cost frequently cross local jurisdiction and may become a national problem [1]. Landslides, resulting from disturbance in slope equilibrium induced by the movement of a mass of rock, debris or earth down a slope and pose a significant threat to landscapes, infrastructure and human life [2]. Landslides can be labelled into different categories depending on the type of movement and the type of material involved. They may be triggered by several phenomena; the primary are seismic activities and heavy rainfall. More precisely, rainfall-induced landslides typically occur in regions prone to heavy precipitation, with steep slopes and poorly consolidated soil or rock [2]. In Italy, the most recent case study, is the Cormons (Gorizia, Italy) landslide occurred on November 17th 2025. Here, intense rainfalls caused a mud-flow inducing the collapse of several buildings and two casualties. In this area, landslides are the most frequent type of instability. These are mostly small and medium-sized landslides, located on flyschoid hills, affecting vineyards and only locally affecting roads and rural settlements [3]. Identifying these phenomena through satellite-based remote sensing techniques offers essential data and insight for landslide studies. Information regarding timing, location and spatial extent of detected landslides, along with changes in surface materials, plays a key role in risk and susceptibility assessments as well as in effective disaster management, monitoring and response activities. For the purpose of this work, optical satellite images provided by Sentinel-2, together with the Lidar provided by the Italian Civil Defense have been used with the aim to identifying the Cormons landslide and its characteristics in terms of dimensions, shape and amount of material moved during the event. The use of optical imagery from Sentinel-2 it’s been used to evaluate spectral indices like Normalized Difference Vegetation Index (NDVI), Normalized Difference Water Index (NDWI) and Bare Soil Index (BSI). Instead Lidar and DEM have been used to define the ground changes in terms of elevation and also the amount of material involved in the event. From the GIS analysis, the results confirm the presence of a mudflow within a watershed located in the Cormons area. Additionally, from the Lidar other small collapse features have been highlighted in the surrounding area.

 

REFERENCES:

  • Highland, L. M., & Bobrowsky, P. (2008). The landslide handbook-A guide to understanding landslides(No. 1325). US Geological Survey.
  • Peters, S., Liu, J., Keppel, G., Wendleder, A., & Xu, P. (2024). Detecting coseismic landslides in GEE using machine learning algorithms on combined optical and radar imagery. Remote Sensing16(10), 1722.
  • https://www.isprambiente.gov.it/files/pubblicazioni/rapporti/rapporto-frane-2007/Capitolo_11_Friuli_Venezia_Giulia.pdf

 

How to cite: scalabrini, A., fornasari, S. F., and costa, G.: Cormons landslide characterization using Lidar and remote sensed data., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6955, https://doi.org/10.5194/egusphere-egu26-6955, 2026.

EGU26-7148 | ECS | Orals | NH3.3

Automated quasi-3D reconstruction of landslide slip surfaces using UAV-derived surface displacement 

Shigeru Ogita, Shoutarou Sanuki, Kazunori Hayashi, Keita Itou, Shinro Abe, Dang Dai Nam Nguyen, and Ching-Ying Tsou

Rapid and safe identification of slip-surface geometry is essential for efficient landslide investigation and mitigation. Conventional approaches to slip-surface determination rely primarily on borehole surveys and in situ instrumentation; however, these methods require long investigation periods and substantial labor.

In this study, we propose a new method that automates slip-surface reconstruction using high-density ground-surface displacement vectors derived from multi-temporal topographic data collected by a laser-equipped UAV at two landslides developed in Neogene formations in northeastern Japan. The analysis estimates two-dimensional slip-surface profiles along multiple cross sections (following Ogita et al., 2024), which are subsequently integrated to construct a quasi–three-dimensional slip-surface geometry. For validation, the landslide moving mass volumes estimated using the proposed method were compared with those identified from dense borehole data. The results show agreement rates of 87% and 96%, respectively. These findings demonstrate that the proposed method achieves sufficient accuracy for practical application in future landslide mitigation planning.

 

References:

OGITA, S., HAYASHI, K., ABE, S., TSOU, C.-Y. (2024): Estimation of slip surface geometry from vectors of ground surface displacement using airborne laser data : case studies of the Jimba and Tozawa landslides in Akita Prefecture, Journal of the Japan Landslide Society, 61(4) 123-129 (in Japanese with English abstract).

How to cite: Ogita, S., Sanuki, S., Hayashi, K., Itou, K., Abe, S., Nguyen, D. D. N., and Tsou, C.-Y.: Automated quasi-3D reconstruction of landslide slip surfaces using UAV-derived surface displacement, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7148, https://doi.org/10.5194/egusphere-egu26-7148, 2026.

EGU26-9556 | Orals | NH3.3

Framework for early detection and characterisation of hydraulically induced shallow landslides 

Mateja Jemec Auflič, Matej Maček, Jasna Smolar, Karin Kure, Tina Peternel, Helena Grčman, Rok Turniški, Marko Zupan, Vesna Zupanc, Luka Žvokelj, and Boštjan Pulko

Shallow landslides triggered by intense and prolonged precipitation represent a major geohazard in many soil-dominated landscapes. This study presents the development of an integrated monitoring and modelling framework for the early detection and characterisation of hydraulically induced shallow landslides. The approach is based on the selection of three representative pilot sites and the implementation of comprehensive field investigations (engineering-geological, pedological, geotechnical, hydrological) and laboratory testing to determine the chemical, physical, and mechanical properties of characteristic soil horizons. A real-time monitoring system has been established to continuously record  soil volumetric water content and suction, together with precipitation, providing high-resolution hydro-meteorological and hydrological data. Geoelectrical measurements and field investigations were applied to characterise soil structure and depth, and to establish relationships between geophysical parameters and physico-mechanical soil properties. These analyses enable the development of a non-invasive monitoring approach capable of diagnosing landslide initiation, delineating landslide geometry, and estimating potentially unstable volumes. Based on the monitoring data obtained at pilot sites, hydro-meteorological thresholds and critical soil parameters controlling shallow landslide occurrence are derived for key soil types. Safety factors and probabilistic landslide occurrence models are developed to identify dominant triggering mechanisms. The results contribute to a national-scale framework for shallow landslide susceptibility mapping and provide a transferable methodology for operational landslide early-warning systems. This research is supported by the Slovenian Research and Innovation Agency through research projects: A holistic approach to Earth surface processes driven by extreme weather events (J7-60124) and Geospatial information technologies for a resilient and sustainable society (GC-0006).

How to cite: Jemec Auflič, M., Maček, M., Smolar, J., Kure, K., Peternel, T., Grčman, H., Turniški, R., Zupan, M., Zupanc, V., Žvokelj, L., and Pulko, B.: Framework for early detection and characterisation of hydraulically induced shallow landslides, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9556, https://doi.org/10.5194/egusphere-egu26-9556, 2026.

EGU26-10241 | Posters on site | NH3.3

Multi-instrument geophysical monitoring of a km-scale slow-moving landslide in Nepal: Technical insights and preliminary results 

Maxime Jaspard, Jérôme Lave, Bhairab Sitaula, Julien Barrière, Ananta Gajurel, and Tanka Paudel and the Team Slide

Himalayan slopes are highly exposed to landslides, primarily triggered by earthquakes and monsoon precipitation. Satellite methods offer unrivalled spatial coverage of surface displacements on a weekly scale. However, they do not directly provide details of deformation at depth, nor do they offer sufficient temporal resolution to elucidate the continuity or intermittent nature of the landslide deformation during phases of heavy rainfall, strong rise in the water table or during intermediate seismic shaking. To address these issues in the context of the ANR/FNR project "SLIDE", we have recently deployed in late October 2025 a geophysical network at the level of one active, km-scale cultivated landslide in Nepal consisting in 16 co-located seismic and GNSS stations and one metereological station.

In this presentation, we will present the practical aspects of deploying and maintaining these instruments in remote Himalayan terrain. Each system required specific installation techniques and careful site selection to ensure stable measurements and long-term performance. Field operations were challenged by difficult access, variable road conditions, limited power availability, and unpredictable weather. Beyond technical challenges, community engagement is essential and close collaboration with local residents guided several site choices. We will also show the preliminary analysis of seismic, GNSS and meteorological data over the first 6 months of operation, which will be applied in the next three years to derive temporal and spatial changes of the landslide properties.

How to cite: Jaspard, M., Lave, J., Sitaula, B., Barrière, J., Gajurel, A., and Paudel, T. and the Team Slide: Multi-instrument geophysical monitoring of a km-scale slow-moving landslide in Nepal: Technical insights and preliminary results, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10241, https://doi.org/10.5194/egusphere-egu26-10241, 2026.

EGU26-10608 | Orals | NH3.3

Deep Learning-Based Assessment of Slope Creep Vulnerability Using Geophysical Survey Data 

Taeho Bong, Jihun Jeon, Eunsoo Jeong, Sieun Lee, Joon Heo, and Jungil Seo

Slope creep refers to the imperceptibly slow and gradual downslope movement of soil and rock driven by gravity. It is mainly driven by moisture-induced expansion of clay-rich materials and the resulting decrease in shear strength. Although subsurface conditions can influence slope creep vulnerability, identifying their effects remains challenging. In recent years, electrical resistivity and seismic surveys have been widely used to characterize the spatial and temporal variability of subsurface soil properties. These geophysical methods provide a non-destructive means of investigating subsurface physical characteristics. In this study, electrical resistivity and seismic surveys were conducted to assess slope creep vulnerability associated with subsurface conditions. Geophysical survey data were obtained from 124 slope sites, and their slope creep vulnerability was classified into two groups (low and high) based on field investigations. Cross-plot analysis was applied to integrate electrical resistivity and seismic velocity, and the resulting data points were classified into four quadrants according to threshold values of seismic velocity and electrical resistivity. The threshold values were statistically determined using a t-test. The composition ratios of the four quadrants were used as input variables for deep learning training, and the bedrock proportion based on seismic velocity included as an additional input. As a result, a total of five input variables were used, and deep learning training was performed by classifying slope creep vulnerability into two groups. As a result, a total of five input variables were used to train a deep learning model for classification of slope creep vulnerability into two groups. Due to the limited dataset size, five-fold cross-validation was applied for model evaluation. As a result, the deep learning model achieved an accuracy of 81.5% and a recall of 83.0% in classifying slope creep vulnerability, indicating its effectiveness in identifying slope creep–prone areas.

 

Acknowledgments: This study was carried out with the support of ´R&D Program for Forest Science Technology (RS-2025-02213490)´ provided by Korea Forest Service (Korea Forestry Promotion Institute).

 

How to cite: Bong, T., Jeon, J., Jeong, E., Lee, S., Heo, J., and Seo, J.: Deep Learning-Based Assessment of Slope Creep Vulnerability Using Geophysical Survey Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10608, https://doi.org/10.5194/egusphere-egu26-10608, 2026.

Under the combined effects of Tibetan Plateau uplift and global climate warming, the transition zone between the northeastern Tibetan Plateau and the Loess Plateau has become one of the most landslide-prone regions worldwide. Intense tectonics, abundant material supply, and densely developed faults produce landslides with large volumes, multi-stage evolution, and complex failure mechanisms, posing severe threats to infrastructure and human safety. However, progressive deformation processes and multi-scale controls remain poorly understood.

This study investigates the Lade–Lijiaxia landslide using an integrated “space–air–ground–subsurface” framework. Field investigations, systematic mapping of cracks and rupture surfaces, high-resolution remote sensing, SBAS-InSAR monitoring (140 SAR images), XRD mineralogical analysis, and SEM observations are combined to elucidate the landslide’s structural features, time-dependent deformation, and material basis.

Results indicate: (1) The landslide’s spatial distribution, boundaries, and internal structure are strongly controlled by regional tectonics. It develops along tectonically weakened zones, with the main sliding direction aligned with dominant lineaments. The landslide comprises a distinct sliding block and a creeping block (~1.5 × 10⁸ m³), representing a tectonically controlled progressive failure mode; (2) Crack and rupture surface analysis shows dominant crack orientations of ~30° and 125°, and rupture dip directions of 130°, 310°, and 20°, reflecting rear scarp tension, internal creep, and sliding surface geometry; (3) SBAS-InSAR indicates slow deformation, with the creeping block reaching ~170 mm/yr, accelerating seasonally during summer–autumn and warm spring due to rainfall and freeze–thaw cycles; (4) XRD reveals vertical heterogeneity: clay content is ~22% in the upper Quaternary deposits and ~38% in underlying Miocene mudstone, dominated by illite. SEM shows localized clay enrichment, fragmented microstructures, and well-developed pores, providing microstructural evidence for long-term creep and strength reduction.

Overall, long-term deformation is primarily controlled by deep-seated tectonics and lithology, while shallow deformation is triggered by seasonal hydrothermal processes. These results improve understanding of progressive failure and creep evolution of large landslides at the northeastern Tibetan Plateau margin and provide insights for hazard assessment and long-term monitoring in the plateau–loess transition zone.

Map of Location Study Area

Geological Map of Study Area

How to cite: Jingqi, Z. and Genhou, W.: Deformation Characteristics and Mechanisms of a Large Landslide at the Northeastern Margin of the Tibetan Plateau Based on Multi-source Data Integration: A Case Study of the Lade–Lijiaxia Landslide, Qinghai Province, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11055, https://doi.org/10.5194/egusphere-egu26-11055, 2026.

EGU26-11274 | ECS | Orals | NH3.3

Exploring the stability of shallow landslides through global sensitivity analysis: a proof of concept from western Rwanda 

Martina Zanetti, Alberto Armigliato, Cesare Angeli, Filippo Zaniboni, Sylvain Barayagwiza, and Catherine Meriaux

Shallow landslides represent a major hazard in western Rwanda, where steep slopes, deeply weathered materials and intense precipitation frequently interact. This study, carried out in the framework of the WALL project (Grant ID: GCRW-CL001, https://www.wallatrwanda.org/), focuses on a landslide-prone area within the Karongi District and presents a proof-of-concept analysis aimed at investigating the sensitivity of slope stability to key geotechnical and pore pressure–related parameters.

Slope stability is analysed using Scoops 3D (Reid et al., 2015), which implements three-dimensional limit-equilibrium methods (LEM) and evaluates slope stability by testing a large number of potential spherical trial failure surfaces. This approach allows for a systematic exploration of potential instability mechanisms while maintaining a computationally efficient framework suitable for regional-scale and data-scarce applications. Due to the limited availability of site-specific geotechnical data, model parameters are defined within plausible ranges derived from published literature and regional information.

Under these conditions, a global sensitivity analysis based on Sobol indices (Saltelli and Sobol, 1995) represents a suitable and robust strategy to investigate model behaviour and uncertainty. The Sobol analysis is applied to investigate the influence of key geotechnical parameters, including cohesion, internal friction angle and unit weight, and additional pore pressure accounting for hydrological conditions on slope stability results. Both first-order effects and higher-order interaction terms are analysed, providing insights into the combined mechanical and hydraulic controls on slope stability.

The proposed workflow identifies the dominant sources of variability on the output and offers a structured basis for prioritizing the quantification of geotechnical parameters in future data acquisition and model refinement, also in connection with specific triggering factors relevant for the studied area, such as rainfall.

 

 

REFERENCES

Reid, M. E., Christian, S. B., Brien, D. L., & Henderson, S. T. (2015). Scoops3D: software to analyze 3D slope stability throughout a digital landscape (No. 14-A1). US Geological Survey.

Saltelli, A., Sobol’, I. M. (1995). Sensitivity analysis for nonlinear mathematical models: numerical experience. Matematicheskoe Modelirovanie, 7(11), 16–28.

How to cite: Zanetti, M., Armigliato, A., Angeli, C., Zaniboni, F., Barayagwiza, S., and Meriaux, C.: Exploring the stability of shallow landslides through global sensitivity analysis: a proof of concept from western Rwanda, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11274, https://doi.org/10.5194/egusphere-egu26-11274, 2026.

EGU26-13251 | ECS | Posters on site | NH3.3

Multi-methodology characterisation  of low energy landslide : Example of Blamécourt (Vexin region, France) 

Gautier Vandecapelle, Philippe Robion, Raphael Antoine, Pauline Souloumiac, Cecile Finco, Frederic Lacquement, Pascale Leturmy, Francois Betard, and Dominique Frizon-de-Lamotte

Landslides are commonly investigated in mountainous regions characterized by steep slopes. In contrast, the low-plateau region of the French Vexin (Paris Basin) is shaped by slopes resulting from  ancient low-energy mass movements. The objective of this study is to describe the geometry and outcrops of an ancient landslide in order to obtain data to geologically characterize its dynamics and processes. In the French Vexin area, valleys are incised into a limestone plateau whose multilayered stratigraphy - comprising coarse limestone, fine sand and clay - controls the water table position. This water table can induce  seepage erosion within the sand layers  beneath  the limestone layers and can be considered as a predisposing factor. This leads to their fragmentation (rotational blocks) and/or their progressive dipping (i.e. cambering) towards the valley bottoms to adapt to the topography subjected to gravitational constraints. 

Recent studies conducted in a similar geological setting in the Champagne vineyards in France have improved our understanding of the links between these mass movements, substrate properties and hydrogeological conditions. However, the French Vexin region exhibits distinctive characteristics: the upper limestone layer is particularly thick and densely fractured, resulting in slope shapes that have never been studied before. 

A representative site in Blamécourt (Magny-en-Vexin, Val d’Oise) was investigated to develop methodology for characterizing slope processes and their geological context. The area includes  three disused quarries, multiple outcrops and a complex morphology. Field observations, high-resolution LiDAR, GIS mapping and electrical geophysical data were combined to analyse this complex landslide. Detailed morphological studies and characterization of geological structures in quarries beneath the plateau have revealed the state of the rock without the influence of the valley. The limestone blocks are fractured in two directions of tectonic origin, corresponding to the regional structural directions. From the plateau edge, a third structural trend aligned with the valley orientation is observed. These three structural directions persist downslope to the base of the slope, as confirmed by field observations and structural analysis. The limestone blocks covering the slope have therefore been affected by gravitational movements, whose structural boundaries result from the combined influence of inherited faults and newly formed structures.

How to cite: Vandecapelle, G., Robion, P., Antoine, R., Souloumiac, P., Finco, C., Lacquement, F., Leturmy, P., Betard, F., and Frizon-de-Lamotte, D.: Multi-methodology characterisation  of low energy landslide : Example of Blamécourt (Vexin region, France), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13251, https://doi.org/10.5194/egusphere-egu26-13251, 2026.

EGU26-13476 | ECS | Posters on site | NH3.3

Hydrological links between shallow and deep zones in a flysch landslide revealed by repeated FDEM surveys and 3D AMT imaging 

Szymon Oryński, Artur Marciniak, Sebastian Kowalczyk, Adrian Flores-Orozco, and Mariusz Majdański

The interplay between internal structure, deformation mechanisms, and subsurface hydrogeological processes controls the long-term stability of large landslides. A key unresolved issue is whether infiltrating groundwater is confined to the landslide body or can migrate into the underlying bedrock along deep-seated structural discontinuities. This problem is particularly relevant in areas underlain by steeply dipping flysch formations, where structural anisotropy may promote vertical groundwater connectivity and influence landslide reactivation. This study focuses on the Cisiec landslide in the Żywiec district of southern Poland, aiming to identify groundwater percolation pathways and their relationship to slope deformation. The landslide affects a ski slope located in a forest–meadow transition zone and moves predominantly east–northeast, with an elevation difference of approximately 100 m. Previous monitoring indicated complex kinematics but did not resolve the depth extent of groundwater infiltration or its coupling with deep geological structures.

We apply an integrated electromagnetic approach explicitly designed to resolve processes across complementary depth ranges. Shallow groundwater dynamics were monitored using time-lapse Frequency Domain Electromagnetics (FDEM), which is sensitive to depths of approximately 0–3 m and was repeated over a three-year interval. FDEM conductivity variations were used to map spatial and temporal patterns of near-surface water percolation within the landslide body. In addition, the in-phase component of the FDEM signal was exploited to detect positional changes of buried infrastructure on the ski slope. When combined with high-precision Differential GPS (DGPS) measurements, these data provided quantitative constraints on surface displacement and landslide activity. To resolve the intermediate-depth range and provide robust constraints for deep imaging, Electrical Resistivity Tomography (ERT) was conducted along five profiles across the landslide. The resulting resistivity sections, which image the subsurface to approximately 30 m depth, were incorporated as a priori resistivity constraints and starting models for the inversion of Audio-Magnetotelluric (AMT) data. This constrained inversion strategy significantly reduced ambiguity in the AMT results and ensured consistency between shallow, intermediate, and deep resistivity structures.

AMT imaging extended the investigation below 30 m depth and enabled the construction of a three-dimensional resistivity anomaly model of the landslide and its geological basement. The model reveals pronounced, near-vertical resistivity structures associated with the Carpathian flysch beneath the landslide, interpreted as preferential pathways for deep groundwater migration. The integrated interpretation of FDEM, ERT, and AMT data indicates that infiltrating groundwater is not restricted to the landslide mass but can penetrate into the bedrock along steeply oriented discontinuities. This hydrogeological connectivity between shallow infiltration zones and deep structural features provides a plausible mechanism for delayed landslide reactivation and long-term slope instability. The study highlights the importance of multi-scale, constraint-driven electromagnetic imaging for improving hazard-relevant conceptual models of complex landslide systems.

How to cite: Oryński, S., Marciniak, A., Kowalczyk, S., Flores-Orozco, A., and Majdański, M.: Hydrological links between shallow and deep zones in a flysch landslide revealed by repeated FDEM surveys and 3D AMT imaging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13476, https://doi.org/10.5194/egusphere-egu26-13476, 2026.

EGU26-14001 | Posters on site | NH3.3

The 3-D anatomy of the Cuolm da Vi slope instability 

Cedric Schmelzbach, Tjeerd Kiers, Nils Chudalla, Florian Amann, and Yves Bonanomi

Cuolm da Vi (CdV) is a deep-seated gravitational slope deformation in central Switzerland with an estimated unstable volume of around 150 million m3. In the central part, surface displacement rates are on the order of 10 to 20 cm/yr. The ongoing south-westward deformation, which is dominated by toppling, is expressed by scarps, graben-like structures, tension cracks, and local instabilities. These landforms suggest gravitational movement guided by inherited tectonic structures. Despite detailed geomorphological mapping, geological-geotechnical investigations, and more than two decades of surface-displacement monitoring, fundamental uncertainties remain regarding, for example, the maximum depth of the unstable mass and the internal deformation processes.

Here, we integrate multiple geophysical and geological constraints into a 3-D structural model of the instability. To establish the model, we combined a 3-D P-wave velocity volume from first-arrival travel-time tomography, microseismicity detected during five months of continuous distributed acoustic sensing (DAS) monitoring, and distributed strain sensing (DSS) observations from around two years of periodic measurements, together with detailed mapping of tectonic features and available geotechnical information. We feed the geophysical and geological data into a 3-D structural and probabilistic geological modelling framework to establish a complex model of the structural features of CdV. The model covers about 1 km² at the surface and extends to a few hundred meters depth.

Low P-wave velocities (Vp < 2000 m/s) spatially coincide with mapped unstable terrain, indicating that velocity variations can help delineating comparatively intact versus more fractured/damaged rock volumes. Based on the geometry of the low-velocity domain, the maximum depth of the unstable mass in the central part is estimated at about 180-200 m. Microseismicity is concentrated within low-velocity regions and clusters near mapped tectonic features, consistent with deformation localized on key planar discontinuities. Key tectonic features are also associated with distinct DSS strain events. The resulting 3-D “static” model provides a quantitative framework for future analyses of temporal changes in microseismicity, with direct relevance for process understanding and the continued development of early-warning strategies at CdV.

How to cite: Schmelzbach, C., Kiers, T., Chudalla, N., Amann, F., and Bonanomi, Y.: The 3-D anatomy of the Cuolm da Vi slope instability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14001, https://doi.org/10.5194/egusphere-egu26-14001, 2026.

EGU26-14514 | ECS | Orals | NH3.3

From Sliding to Flowing: Integrating Geotechnical, Mineralogical, and Rheological Controls on Earthflow Mobility 

Mariagiulia Annibali Corona, Domenico Calcaterra, Nicola Antonio Di Spirito, Francesco Izzo, Alessio Langella, Mariano Mercurio, Rossana Pasquino, Giacomo Russo, Enza Vitale, and Luigi Guerriero

Earthflows are flow-like landslides involving fine-grained, clay-rich materials that exhibit complex kinematics, long-term activity, and alternating phases of slow movement and sudden acceleration. Although their flow-like behaviour is commonly attributed to distributed internal deformation and plastic rheology, the mechanisms governing the transition from solid-like sliding to fluid-like flowing remain poorly understood, particularly with respect to boundary conditions and material properties. This transition is critical, as it may lead to surging events associated with high mobility and significant hazard.
This study investigates the role of mineralogical, geotechnical, rheological, and geomorphological factors in controlling earthflow mobility and material fluidization. A set of representative earthflows located in the southern Apennines was selected, covering a wide range of geological settings and morphological characteristics. Laboratory analyses were conducted on samples collected from different sectors of the landslides, including grain size distribution, Atterberg limits, mechanical behaviour, quantitative mineralogical composition. Moreover, rheometrical analysis of the fine fractions under controlled shear conditions were also performed. These data were integrated with long-term geomorphological analyses based on satellite imagery and morphometric reconstructions of landslide geometry.
Earthflow behaviour was analysed using a one-dimensional framework based on a Herschel–Bulkley viscoplastic rheological model, aimed at reproducing internal kinematic compartmentalisation in relation to variable water content.
The influence of water content variations, as a function of rainfall-induced infiltration conditions, on rheological parameters and mechanical response was investigated. The results highlight strong correlations between plasticity, occurrence of expandable clay minerals, rheology, and mobility, emphasizing the key role of fine-grained materials in promoting solid–fluid transitions. 
By integrating multi disciplinary datasets, this work advances the understanding and prediction of earthflow fluidization and mobility-processes for which current forecasting capabilities remain notably limited.

How to cite: Annibali Corona, M., Calcaterra, D., Di Spirito, N. A., Izzo, F., Langella, A., Mercurio, M., Pasquino, R., Russo, G., Vitale, E., and Guerriero, L.: From Sliding to Flowing: Integrating Geotechnical, Mineralogical, and Rheological Controls on Earthflow Mobility, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14514, https://doi.org/10.5194/egusphere-egu26-14514, 2026.

EGU26-14669 | ECS | Orals | NH3.3

Experimental constraints on the slip response of a slow-moving landslide to rainfall driven pore pressure changes 

Kaitlin Schaible, Demian Saffer, and Noah Finnegan

Landslide motion spans a continuum from slow, steady creep to rapid catastrophic failure. However, the mechanisms controlling the timing, rate, and nature of sliding, the sensitivity of motion to perturbations driven by precipitation or human activity, and potential transitions from creep to catastrophic failure all remain poorly understood. The response of landslide basal shear zones to rainfall-driven changes in pore pressure and thus effective stress can be interpreted using rate and state friction, a framework that describes the constitutive behavior and sliding stability of frictional shear zones, and is widely applied to earthquake mechanics. Laboratory experiments provide direct constraints on these frictional properties, and thus hold the potential to illuminate the material properties and conditions that control basal slip. We investigate the frictional behavior of Oak Ridge earthflow, a slow-moving landslide in the Coast Ranges of central California hosted within a clay-rich mélange. We conduct a suite of direct shear experiments to characterize its frictional rheology, including both (1) the velocity dependence of friction measured from velocity step tests; and (2) frictional healing, or time-dependent restrengthening between slip events, measured via slide-hold-slide tests. Experiments are conducted across a range of normal stresses approximating the in-situ conditions of the active shear plane (0.3 – 2 MPa) and at sliding velocities that span the range of observed landslide creep (0.001 – 30 𝜇m/s).

The shear plane material exhibits uniformly velocity strengthening behavior, characterized by a positive rate parameter (a-b), indicating that friction increases with increased slip rate, and is consistent with stable sliding. The values of (a-b) from laboratory experiments ranges from 0.001 – 0.015, in agreement with values inferred from coupled field observations of slide motion and pore pressure. Our results suggest that velocity strengthening friction, combined with modulation of effective stress through pore pressure, can generate slip transients, providing a direct mechanistic link between laboratory scale behavior and field observations of landslide motion.

We also find that the clay rich materials entrained along the base of the slide exhibit little to no healing (𝛽 ≈ 0). Near zero healing implies that the slide does not restrengthen during extended periods of low water pressure during the dry California summer. In the absence of healing, slip velocity responds directly and immediately to changes in pore pressure, independent of the duration of dry periods. Taken together, velocity strengthening friction and little to no healing are consistent with the persistent creep observed in the field, where the slip rate is governed by the stress state, pore pressure, and rate dependence of friction. Notably, Oak Ridge earthflow has been active since at least the 1930’s (the date of first air photos). The laboratory derived frictional rheology provides a quantitative framework to explain the observed landslide slip response to changes in pore pressure and suggests that friction laws can be used not only to interpret past slide behavior, but potentially to predict landslide responses to future climate-driven hydrologic forcing or other external perturbations.

How to cite: Schaible, K., Saffer, D., and Finnegan, N.: Experimental constraints on the slip response of a slow-moving landslide to rainfall driven pore pressure changes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14669, https://doi.org/10.5194/egusphere-egu26-14669, 2026.

Relative seismic velocity changes (dv/v) derived from ambient noise interferometry serve as a proxy for the internal rigidity or structural health of landslide materials. Strong ground motion often induces coseismic velocity drops, indicating damage within the shallow crust or the landslide body. This study focuses on the deep-seated, slow-moving Wuhe landslide in eastern Taiwan, which exhibits stable creeping with daily displacement rates ranging from 4 mm to 25 mm(Weng et al., 2025), to investigate its response to the September 2022 earthquake sequence, specifically the ML 6.6 Guanshan and ML 6.8 Chihshang earthquakes.To monitor temporal variations in the landslide's internal state, we applied the single-station cross-component (SC) technique to the Wuhe landslide using continuous ambient noise records. The seismic monitoring network comprises one geophone installed directly on the sliding mass and three reference stations located on stable bedrock outside the landslide area. This configuration aims to differentiate between landslide-specific structural changes and regional reference variations. The preliminary results showed that a clear seismic velocity reduction was found spatially within the landslide area. Through dv/v measurements with in-situ real-time kinematic (RTK) GPS data and strong-motion records, the coseismic velocity drops are in response to the accelerating surface displacement and strong ground shaking, and the spatial relationships between dv/v, surface movement and peak-ground acceleration (PGA) are systematically compared . In fact, the earthquake did not trigger catastrophic landsliding at the Wuhe site, Thus, we further investigate the recovery of landslide material properties following strong ground shaking. The post-seismic recovery duration captured by dv/v observations can help us to better understanding recovery mechanism of landslide material after earthquakes.

How to cite: Weng, H.-K. and Chao, W.-A.: Coseismic Seismic Velocity Variations of a Deep-Seated Landslide Caused by Two M6.5+ Earthquakes in Eastern Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15810, https://doi.org/10.5194/egusphere-egu26-15810, 2026.

EGU26-16829 | Orals | NH3.3

Linking Hydrological Forcing to Seismic Sensitivity in an Unsaturated Slope Using Physics-Based Modelling 

Thomas Dylan Mikesell, Emma Brennvall Lorentzen, Luca Piciullo, and Mathilde Bøttger Sørensen

With intensifying precipitation events, landslides pose increasing environmental hazards. Unsaturated slopes are key monitoring targets due to their rapid, and sometimes severe, response to rainfall. This study investigates how hydrological changes in an unsaturated slope in Eidsvoll (Norway) influence seismic velocities through time and space using a physics-based modelling framework. Vertical effective stress and density fields from hydromechanical simulations in GeoStudio are used as inputs to the Biot-Gassmann relationship to estimate time-varying P- and S-wave velocities. These velocities are used to compute Rayleigh wave phase velocity dispersion curves and sensitivity kernels for selected days throughout a 250-day (September 2019-May 2020) simulation period. The results reveal a strong coupling between infiltration, effective stress, and seismic velocities, especially in the upper part of the unsaturated slope. Rayliegh wave sensitivity is highly frequency- and depth- dependent: high frequencies (above 60 Hz) are sensitive to near-surface changes, while lower frequencies probe deeper layers. A persistent blind zone in an intermediate high-velocity layer limits the surface waves sensitivity to certain depths, underscoring the importance of survey design and the usefulness of surface waves depending on the geologic scenario. This forward modelling approach enables identification of optimal frequency ranges and target depths, providing critical input for future field investigations. These findings contribute to the development of focused site-specific seismic monitoring strategies, including passive surveys using anthropogenic noise sources or active source MASW. By bridging hydromechanical modelling and the associated seismic response using slope-scale physical processes, this approach can support early warning systems and landslide hazard assessment under changing climate conditions.

How to cite: Mikesell, T. D., Lorentzen, E. B., Piciullo, L., and Sørensen, M. B.: Linking Hydrological Forcing to Seismic Sensitivity in an Unsaturated Slope Using Physics-Based Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16829, https://doi.org/10.5194/egusphere-egu26-16829, 2026.

EGU26-17167 | ECS | Posters on site | NH3.3

Unveiling the role of seepage forces in the acceleration of frictional creep in fluid-saturated shear zone 

Fabian Barras, Andreas Aspaas, Einat Aharonov, and François Renard

How fluid impact frictional slip is a central question in various geological settings, from tectonic faults to friction at the base of glaciers. In this work, we study the impact of fluid infiltration on the creep dynamics of the shear zone located at the base of a densely monitored landslide in Western Norway. In Åknes, approximately 50 million cubic meter of rock mass continuously creeps over a shear zone made of rock fragments, with seasonal accelerations that strongly correlate with rainfall. In this natural laboratory for fluid-induced frictional creep, unprecedented monitoring equipment reveals low fluid pressure across the shear zone, thereby challenging the conventional theory of fluid-driven instability in landslides. Here, we show that a generic micromechanical model can disentangle the effects of fluid flow from those of fluid pressure, and demonstrate that seepage forces applied by channelized flow along the shear zone are the main driver of creep accelerations. We conclude by discussing the significance of seepage forces, the implications for hazard mitigation and the broader applicability of our model to various geological contexts governed by friction across saturated shear zones.

How to cite: Barras, F., Aspaas, A., Aharonov, E., and Renard, F.: Unveiling the role of seepage forces in the acceleration of frictional creep in fluid-saturated shear zone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17167, https://doi.org/10.5194/egusphere-egu26-17167, 2026.

EGU26-17252 | Posters on site | NH3.3

Rapid estimation of block volumes from seismic noise measurements and an eigenfrequency abacus  

Veronica Pazzi, Simone Francesco Fornasari, Stefano Devoto, Giovanni Costa, and Emanuele Forte

Estimating the volume of potentially unstable rock masses is a critical yet challenging task in landslide characterization. Traditional methods often struggle to accurately define the height and actual separation of rock blocks because of the hidden nature of fracture persistence. In engineering geology and geophysics, natural frequency (f0) refers to the fundamental modes of vibration of materials, rock masses, soil layers, entire slopes, as well as different man-made structures. A variety of studies have explored the natural frequency and resonance phenomena across contexts using both experimental and numerical approaches.

This work is based on the principle that specific peaks in the Horizontal to Vertical Spectral ratio (H/V) curves of rock blocks are linked to their eigenfrequencies rather than stratigraphic resonance proposes. These frequencies are characterized by strong polarization and linearity normal to the fracture network. Thus, the frequency (fHV) estimated from H/V measurements, is considered a good approximation/estimator of f0 (the block eigenfrequency) and an innovative approach to estimate block volumes from an abacus is proposed. The eigenfrequency-volume abacus was build using Finite Element Method (FEM) simulations. Rock blocks were modelled as rectangular cuboids with fixed boundary conditions at the base, similar to an Euler–Bernoulli cantilever. The simulations integrated site-specific mechanical parameters (Young’s modulus, density, and Poisson’s ratio) consistent with a S-wave velocity of approximately 850 m/s.

The procedure was validated using seismic noise datasets from two test sites on Malta Island (Anchor Bay and Il-Qarraba), where independent volume data from UAV-Digital Photogrammetry and satellite imagery were available. The proposed six-step workflow - ranging from data acquisition to the integration into the abacus of fHV with independent surface area (A) measurements - provides a reliable approximation of the volume's order of magnitude, even with errors in frequency selection.

A key advantage of this method is the ability to use easily obtainable seismic noise data to infer structural properties. Furthermore, discrepancies between abacus-derived volumes (Vest) and field-calculated volumes (Vcalc) can serve as indicators of fracture persistence: Vest < Vcalc suggests fractures are less persistent than they appear, while Vest > Vcalc indicates higher isolation from the rock mass. While the current abacus is site-specific, the methodology is adaptable to different geological backgrounds. This tool represents a significant step forward for rapid, non-invasive rockfall hazard assessment and the characterization of block-release susceptibility.

How to cite: Pazzi, V., Fornasari, S. F., Devoto, S., Costa, G., and Forte, E.: Rapid estimation of block volumes from seismic noise measurements and an eigenfrequency abacus , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17252, https://doi.org/10.5194/egusphere-egu26-17252, 2026.

EGU26-17460 | ECS | Orals | NH3.3

3D structure and deformation evolution of a large deep-seated toppling revealed by GMM-based multi-source geophysical integration 

Hui Wang, Xiangjun Pei, Zhanjun Quan, Shenghua Cui, Shiping Xing, and Yu Wang

Exploring the internal structure of large landslides is crucial for understanding their deformation mechanisms and conducting stability assessments. However, traditional exploration methods, such as drilling, provide only localized information and fail to reflect the spatial continuity of subsurface structures. Single geophysical methods also face challenges in accurately characterizing deep-seated structures due to inversion non-uniqueness and interpretative ambiguity. Multi-source geophysical data fusion is considered an important approach to reduce ambiguity and improve modeling reliability, but existing research largely focuses on shallow landslides, lacking effective methods for the three-dimensional reconstruction of large deep-seated rock landslides. Taking the Tizicao deep-seated toppling on the eastern edge of the Tibetan Plateau as an example, this study proposes a multi-source geophysical data fusion modeling method based on the Gaussian mixture model (GMM). This method comprehensively utilizes electrical resistivity tomography (ERT), multi-channel surface wave exploration (MASW), the horizontal and vertical spectral ratio method (HVSR) for ambient noise, and UAV photogrammetry to achieve the fusion and classification of multiple parameters such as resistivity, shear wave velocity, and structural depth. By automatically partitioning the geophysical feature space using GMM, a three-dimensional model of the Tizicao toppling is constructed. The three-dimensional model is highly consistent with the borehole results, verifying the reliability of the fusion modeling method. In addition, the deep-seated structure revealed by the three-dimensional model plays a key controlling role in the initiation of slope instability. Overall, the proposed GMM-based multi-source geophysical fusion method not only enables accurate reconstruction of the internal structure of large deep-seated rock landslides but also provides a new technical pathway for mechanism analysis and hazard prediction of large deep-seated landslides.

Keywords: Deep-seated toppling; Multi-source geophysical integration; Gaussian Mixture Model (GMM); 3D structural modeling; Deformation evolution.

How to cite: Wang, H., Pei, X., Quan, Z., Cui, S., Xing, S., and Wang, Y.: 3D structure and deformation evolution of a large deep-seated toppling revealed by GMM-based multi-source geophysical integration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17460, https://doi.org/10.5194/egusphere-egu26-17460, 2026.

Global warming has accelerated glacier retreat and permafrost degradation in high-elevation regions, significantly increasing the frequency and magnitude of glacier-related debris flows. This study focuses on Tianmogou, a debris-flow-prone catchment on the Tibetan Plateau, where three broadband seismometers were deployed for continuous monitoring during the active period. Using ambient noise interferometry, relative seismic velocity changes (dv/v) and the effective decorrelation coefficient (dCe) were calculated to achieve high-resolution characterization of the temporal evolution of subsurface mechanical properties.

The results show that dv/v exhibits pronounced seasonal variations and is significantly negatively correlated with soil temperature, while short-term hydrological processes, such as intense rainfall and snowmelt, lead to rapid dv/v decreases accompanied by marked dCe increases. Notably, several hours prior to multiple debris-flow events, persistent dv/v reductions and rapid dCe increases were consistently observed as precursory signals, with rainfall-triggered events (e.g., 10 July 2020) displaying particularly prominent precursory characteristics. By jointly analyzing seismic velocity changes, precipitation, and soil moisture, this study reveals the progressive degradation of subsurface media during debris-flow initiation and demonstrates the potential of seismic methods for long-term hazard monitoring in glacial and periglacial environments.

How to cite: Lyu, A. and He, S.: Seismic Precursory Velocity Changes Associated with Debris Flows in Tianmogou Inferred from Ambient Noise Interferometry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17858, https://doi.org/10.5194/egusphere-egu26-17858, 2026.

EGU26-17967 | Orals | NH3.3

Assessing Climate-Driven Changes in Rainfall-Induced Landslide Probability Using Distributed Hydrological Modeling 

Elisa Arnone, Juby Thomas, Diego Ciriminna, and Antonio Francipane

Rainfall-induced shallow landslides represent a critical natural hazard in mountainous regions, with their frequency controlled by hydrological processes. Climate change is expected to alter both precipitation patterns and soil moisture dynamics but quantifying these impacts on landslide susceptibility remains challenging.

In this study, we integrate physically-based stability thresholds with distributed hydrological modeling to assess future landslide hazard evolution under multiple climate scenarios. The study is conducted for a small basin (~28 km2) located in the north-eastern Friuli Venezia Giulia (Italy).

Spatially explicit Critical Soil Moisture (CSM) and Critical Wetness Index (CWI) thresholds at 50 m resolution were derived in a previous effort for multiple failure depths (0.75 to 2.00 m) by inverting the infinite slope stability analysis. The thresholds represent hydrological conditions at which slope failure may initiate through either unsaturated zone processes or groundwater table rise. These thresholds were coupled with a calibrated distributed and physically-based hydrological model, the Triangulated Irregular Network‐based real‐time integrated basin simulator (tRIBS), which simulates hourly soil moisture and groundwater dynamics, to assess the occurrence of failure over 100-year periods for three synthetically generated climate scenarios: current conditions, moderate emissions (RCP4.5, 2050), and high emissions (RCP8.5, 2050). The synthetic series of meteorological variables, and particularly precipitation, were generated by combining the AWE-GEN (Advanced WEather GENerator) model with a procedure to correct the distribution of extreme events.

We quantify exceedance frequencies, i.e., the proportion of time during which CSM and CWI thresholds are exceeded, as a measure of temporal exposure to landslide-conducive conditions. Results reveal that, under RCP4.5, exceedance frequencies decrease by up to 14.6% (CWI) and 10.9% (CSM), due to a reduction in annual precipitation despite an increase in mean intensity per event. In contrast, RCP8.5 shows bidirectional patterns, with maximum increases reaching 5.1% (CWI) and 3.6% (CSM), indicating that precipitation intensification begins to overcome the reduction in annual precipitation. Critically, climate impacts amplify with failure depth; the 2.00 m failure depth exhibits changes in magnitude up to three times greater than those at 0.75 m, suggesting that deeper failures become disproportionately more sensitive to climate change.

This research received funding from European Union NextGenerationEU – National Recovery and Resilience Plan (PNRR), Mission 4, Component 2, Investment 1.1 -PRIN 2022 – 2022ZC2522 - CUP G53D23001400006.

How to cite: Arnone, E., Thomas, J., Ciriminna, D., and Francipane, A.: Assessing Climate-Driven Changes in Rainfall-Induced Landslide Probability Using Distributed Hydrological Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17967, https://doi.org/10.5194/egusphere-egu26-17967, 2026.

EGU26-19557 | ECS | Posters on site | NH3.3

Reconstructing rainfall-induced landslides at the global scale 

Yi Xia and Ke Zhang

Rainfall-induced landslides are among the most widespread and destructive natural hazards, yet their physical reconstruction has rarely been explored beyond local or regional scales. We present a simplified slope-stability framework driven entirely by globally available rainfall, soil, and topographic datasets, and demonstrate its ability to reproduce thousands of rainfall-triggered landslides documented in the Global Landslide Catalog (GLC).By avoiding computationally intensive hydrological simulations while retaining physical interpretability, the proposed approach enables large-scale reconstruction of rainfall-induced slope failures across diverse environmental settings. Sensitivity analyses indicate that slope geometry and rainfall forcing primarily control proximity to failure and its timing, whereas soil bulk density exerts a disproportionate influence on model uncertainty due to its structural role in both mechanical resistance and hydrological response.Model performance is strongest in tropical and temperate regions, while reduced skill is observed in arid and cold climates, where failures tend to be conservatively predicted, favouring early-warning applications. Under scenarios characterised by intensified extreme rainfall, the framework suggests an overall increase in global slope instability. These results demonstrate the feasibility of reconstructing rainfall-induced landslides at the global scale using simplified physical representations, and highlight key directions for further improvement, including vegetation effects, subsurface heterogeneity, and hydrological process representation.

How to cite: Xia, Y. and Zhang, K.: Reconstructing rainfall-induced landslides at the global scale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19557, https://doi.org/10.5194/egusphere-egu26-19557, 2026.

EGU26-19964 | ECS | Posters on site | NH3.3

Sensitivity Analysis of Physically-based 3D Landslide Susceptibility Model from Variation of Input Parameters 

Enok Cheon, Marie Gotaas, Sivert Pettersen, Emir Ahmet Oguz, Amanda DiBiagio, and Luca Piciullo

Shallow landslides frequently occur on natural slopes and cause flow-like disasters. The authors have previously developed 3-Dimensional Translational Slide (3DTS), a physically-based 3D shallow landslide susceptibility model accounting for side resistance and vegetation effects, to efficiently evaluate the slope stability in terms of the factor of safety (FS) over a regional scale. Traditionally, a deterministic slope stability analysis was performed by assigning representative values to rainfall history, soil layers, and soil properties; however, new design standards demand reliability-based analyses that account for the uncertainty and variation in precipitation, subsurface conditions, soil hydro-geotechnical properties, and vegetation root reinforcement. Therefore, this research proposes extending the developed model into a 3-Dimensional Translational Slide-Probabilistic (3DTSP) model to enable reliability-based landslide susceptibility assessment. The developed 3DTSP model combines the generalized Green-Ampt infiltration model and the 3D Janbu simplified slope stability model. The 3D slope stability analysis accounts for additional soil frictional resistance at the side regions in translational slides and additional reinforcements from tree roots. The 3DTSP model uses a Monte Carlo simulation with a random-field approach to determine the FS statistical distribution from variations in the following input parameters: soil thickness, hydraulic properties, Mohr-Coulomb criterion-based shear strength properties, unsaturated soil strength properties, and vegetation resistance properties. Based on the statistical distribution and characteristic length, the model generates a random field of input parameters that accounts for spatial variation in the horizontal direction. For each Monte Carlo simulation iteration, a new random input field is generated to compute FS. The performance and applicability of the developed 3DTSP for probabilistic assessment of landslide susceptibility over regional scales were demonstrated by analyzing landslide case studies. A sensitivity study was conducted to assess the sensitivity of FS to variations in soil thickness, soil properties, and vegetation properties.

How to cite: Cheon, E., Gotaas, M., Pettersen, S., Oguz, E. A., DiBiagio, A., and Piciullo, L.: Sensitivity Analysis of Physically-based 3D Landslide Susceptibility Model from Variation of Input Parameters, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19964, https://doi.org/10.5194/egusphere-egu26-19964, 2026.

EGU26-21563 | Posters on site | NH3.3

Mapping Landslide Susceptibility in the Moldavian Plain, Romania 

Radu Irimia, Ionut Sandric, and Viorel Ilinca

Shallow landslides represent a frequent geomorphological process in the study region, located in northeastern Romania. The area is characterized by gently undulating interfluves, fragmented slopes, and deeply incised valleys, developed predominantly on clayey substrates. These predominantly shallow slope failures have significant impacts on intensive agriculture, rural infrastructure, and slope stability. Recent climatic variability and anthropogenic modifications of land use amplify the vulnerability of this geomorphological unit. This study presents a detailed assessment of shallow landslide susceptibility through the integration of an extensive landslide inventory with conditioning factors derived from high-resolution geospatial data. The landslide inventory was developed predominantly using digital elevation models generated from LiDAR data (1–2 m resolution), complemented by current orthophotos, drone aerial imagery, slope maps, and selective field validation. The use of LiDAR data substantially improves the precision of delineating shallow unstable features and reduces propagation errors associated with conventional lower-resolution DEMs. This methodology enabled the precise delineation of hundreds of active and relict shallow landslide features, surpassing the limitations of traditional inventories based on photogrammetry or global DEMs.
Relevant conditioning factors for slope dynamics in this region included slope angle, aspect, plan and profile curvature, lithological units (predominantly Miocene-Pliocene clayey deposits), land use, and distance to the drainage network. The dataset was divided into 70% for calibration and 30% for independent validation. The Presence Only Model performance was evaluated through ROC curves and AUC metrics, with values consistently demonstrating excellent predictive performance of the hybrid approach employed.
Results highlight zones of high and very high susceptibility to shallow landslides concentrated along major valleys and their tributaries, and on slopes exceeding 12–15°, where favourable lithological conditions overlap with intensive agricultural land uses or reduced vegetation cover. Methodologically, this study aligns with established international approaches for landslide susceptibility assessment but distinguishes itself through the use of high-resolution LiDAR data (1–2 m), specifically adapted to the morphological context of the region—an area with gently rolling relief and deeply incised valleys. This choice enables substantial reduction of topographic uncertainties inherent in models based on medium or low-resolution DEMs, thereby improving the precision of shallow instability feature delineation and the robustness of local predictions. The result is a susceptibility model with high transferability potential to other similar geomorphological units in plain-to-hill transition zones affected by shallow landsliding.

How to cite: Irimia, R., Sandric, I., and Ilinca, V.: Mapping Landslide Susceptibility in the Moldavian Plain, Romania, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21563, https://doi.org/10.5194/egusphere-egu26-21563, 2026.

EGU26-22967 | ECS | Orals | NH3.3

Understanding and Zoning Rainfall-Induced Landslide Hazards in Indonesia: Insights from Observation to Forecasting 

Lisa Agustina, Christian Arnhardt, Maximillian Van Wyk De Vries, Ekbal Hussain, David Large, and Barbara Turnbull
As one of the most destructive natural hazards, landslides pose persistent threats to human life, property, and critical infrastructure in Indonesia, where intense rainfall and steep, complex terrain strongly control landslide occurrence and impacts. Although landslides may be triggered by multiple factors, including earthquakes and prolonged rainfall, rainfall remains the only trigger that can be forecasted, making it central to operational landslide early warning. Between 2019 and 2024, based on Indonesian Disaster Information Database (DIBI–BNPB), more than 4,000 landslides were recorded across Indonesia, causing substantial loss of life and widespread damage to housing and public infrastructure.
At present, landslide early warning in Indonesia relies on a single nationwide rainfall threshold, which may limit forecast accuracy and reliability given the country’s strong spatial variability in rainfall patterns and geomorphological conditions. Developing rainfall thresholds at large spatial scales is therefore challenging. To address this limitation, this study adopts a zoning approach that prioritises areas with high landslide susceptibility and potentially severe impacts, providing a targeted basis for subsequent threshold development.
Landslide susceptibility maps are produced using the Analytical Hierarchy Process (AHP), chosen in preference to data-driven methods due to biases and incompleteness in the available landslide inventory, which tends to reflect population distribution rather than true landslide source areas. Two provinces, Central Java and South Sulawesi, are selected as initial case studies. According to the data from Local Indonesian Disaster Management (BPBD), more than 2,000 landslides were recorded in Central Java between 2016 and 2025, while over 500 events were documented in South Sulawesi between 2021 and 2025.
Population density, building distribution, landslide susceptibility, and landslide runout probability are integrated to identify zones with the highest potential impacts. These high-impact zones serve as priority areas for developing more representative rainfall thresholds, with the aim of improving landslide forecasting and risk reduction in Indonesia.

How to cite: Agustina, L., Arnhardt, C., Van Wyk De Vries, M., Hussain, E., Large, D., and Turnbull, B.: Understanding and Zoning Rainfall-Induced Landslide Hazards in Indonesia: Insights from Observation to Forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22967, https://doi.org/10.5194/egusphere-egu26-22967, 2026.

EGU26-2146 | ECS | Orals | NH3.5

Structural and Kinematic Controls on Paraglacial Rock Slope Deformation at Portage Glacier, Alaska 

Emilie Lemaire, Pooya Hamdi, Anja Dufresne, Bretwood Higman, Jane Walden, Andrea Manconi, Mylène Jacquemart, and Florian Amann

As glaciers thin and retreat worldwide, the stability of surrounding rock slopes is increasingly at risk. This study investigates the long-term deformation of two major on-going instabilities, Portage A and Portage B, situated above Portage Glacier in Alaska. By analyzing decades of historical imagery and remote sensing data, we reconstructed the spatial evolution of these slopes, revealing progressive deformation up-glacier over the past sixty years. To further assess the links between glacier change and slope deformation, we combine structural mapping with remote sensing observations and kinematic analyses. Our results identify three distinct kinematic domains and show that progressive deformation is initiated once the glacier surface lowered below a critical elevation. This creates kinematic freedom for the rock mass to move along structural discontinuities. At Portage Glacier, the onset and progression of the instabilities are not governed solely by glacier thinning but reflect a complex, site-specific interaction between structural discontinuities and cumulative weakening from external processes. Glacier retreat and thinning act as one component within a broader “cascade system”, where multiple factors interact. Additionally, preliminary results from our three-dimensional model provide additional insights into the mechanical response of the slopes under changing boundary conditions. These findings highlight the importance of integrating structural, kinematic, and remote sensing data to better understand paraglacial slope dynamics and anticipate future instabilities in rapidly deglaciating mountain regions.

How to cite: Lemaire, E., Hamdi, P., Dufresne, A., Higman, B., Walden, J., Manconi, A., Jacquemart, M., and Amann, F.: Structural and Kinematic Controls on Paraglacial Rock Slope Deformation at Portage Glacier, Alaska, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2146, https://doi.org/10.5194/egusphere-egu26-2146, 2026.

With the rapid development of the national economy, a large number of projects such as highways, railways, and hydropower stations have been constructed in the mid-western mountainous areas of China. The instability and rockfall of dangerous rock masses in engineering areas have become a serious and frequently occurring geological hazard. In order to reduce economic losses caused by the collapse of dangerous rock masses and ensure the safety of people's lives and property, research on the failure and disaster mechanism of dangerous rock masses, the kinematic characteristics during the collapse process, and risk management has become a major technical challenge that urgently needs to be addressed in the field of disaster prevention and mitigation. Taking the sudden falling-type collapse of dangerous rock masses on the steep cliff at Section K35+850 of the Lichuan-Wanzhou Expressway in western Hubei Province as the engineering background, this study employed unmanned aerial vehicle (UAV) photogrammetry technology to acquire the 3D point cloud and 3D realistic model of the dangerous rock masses on the subgrade steep cliff, and extracted the geometric characteristics of the residual dangerous rock masses. Based on the structural plane interpretation technology using the 3D model, the occurrence information of the dangerous rock masses and their controlling structural planes was obtained. Numerical simulations were performed using Rocfall and 3DEC software to deduce the movement trajectories and influence ranges of the residual dangerous rock masses, and a risk assessment was carried out by segmenting the falling area of the dangerous rock masses. Finally, reasonable disposal measures and technical suggestions for the risk management of the dangerous rock masses were put forward.

How to cite: Wang, B.: Research on the Hazard Assessment for Highway Slope Dangerous Rock Masses, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2727, https://doi.org/10.5194/egusphere-egu26-2727, 2026.

EGU26-3573 | ECS | Orals | NH3.5

Back analysis of ice avalanches using depth-averaged modelling 

Andres Felipe Escobar Rincon, Emmanuel Thibert, Mylène Bonnefoy-Demongeot, and Thierry Faug

As climate change continues, many glaciers around the world are warming and melting. Among these glaciers, those located in steep mountains are susceptible to instabilities, increasing the risk of a sudden release of ice. This release of ice may turn into a granular flow as the ice fractures while rolling downhill, sometimes over long distances, posing significant risks to infrastructures and mountain communities at lower altitudes. As the frequency of ice avalanches is expected to increase in the coming decades, it is crucial to understand and estimate their runout distances and the geometry of the final deposit to assess potential threats.
In this study, we simulated 15 past, well-documented ice avalanches with known volumes of detached ice and estimated release and deposition areas. The selected avalanches cover a wide range of volumes, from 40,000 to 85 million cubic meters, and are mainly located in the Alps, with two additional events in the Aru range in China. These avalanches are composed of ice, whereas flows mixed with snow, rocks, or water exhibit a different flow rheology. To simulate the ice avalanches, we used a depth-averaged flow model with the Voellmy rheology. This method is commonly used to reproduce large geophysical flows such as landslides and snow avalanches. For each event, multiple simulations were performed to define the parameter set that reproduces the observed avalanche's runout and geometry. Among these parameters, cohesion is determined based on weather conditions, and the Voellmy friction parameters, dry and turbulent friction, are systematically adjusted. 
From the performed simulations, we found a strong relationship between the volume of the ice avalanche and dry friction, with dry friction decreasing as volume increases. Moreover, turbulent friction is found to depend mainly on flow volume and dry friction, but is also influenced by other factors, such as topography and temperature at the time of the event. These results also provide insight into the internal dynamics of ice avalanches, which align with the few cases for which velocities were estimated. Based on the estimated parameters, we propose a scaling law to simulate an ice avalanche relying on the released ice volume. This study aims to provide an initial set of parameters for estimating the runout and final deposit of ice avalanches, contributing to forecasting and mitigating the risks associated with potential ice avalanches.

How to cite: Escobar Rincon, A. F., Thibert, E., Bonnefoy-Demongeot, M., and Faug, T.: Back analysis of ice avalanches using depth-averaged modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3573, https://doi.org/10.5194/egusphere-egu26-3573, 2026.

EGU26-3801 | Orals | NH3.5 | Highlight

Monitoring of the "Kleines Nesthorn" and of the Birch Glacier before and during the rock avalanche in Blatten 

Maxence Carrel, Johannes Gassner, Janine Wetter, Ólafur Stitelmann, Théo St.Pierre - Ostrander, and Stéphane Vincent

On May 28th 2025, a massive rock avalanche buried the village of Blatten under 9 million m3 of ice and rock. Thanks to the expertise of many specialists and continuous monitoring and data collection from measurement systems in the field, it was possible to detect this danger in advance and to protect the life of many people. Already before this tragedy in Blatten, the movement of the Birch Glacier was monitored. These monitoring systems later also revealed the upcoming collapse of the Kleines Nesthorn and the associated collapse of the glacier. Consulting expert Geoformer and local authorities mandated Geoprevent to install an interferometric radar which was done at the day, when Blatten was evacuated. The radar installed provided valuable data about the displacement of the entire region around the Birch Glacier and helped the authorities to manage the situation. This system records even small movements of the mountain independent of rain, snow, fog or darkness and can therefore see things that a human eye cannot. It can be used up to distances of 5 km and to monitor areas of more than  5 km2. Only one day before the collapse of the glacier Geoprevent installed a camera on the Eastern moraine of the Birch Glacier to monitor it from the top. These images revealed a dramatic picture during the last hours and showed a rapid movement of the glacier, with measured velocities of several tens of meters per day in the hours leading to the collapse of the glacier. With this camera-based technology and the help of complex algorithms, our monitoring system was able to provide data about the displacement to the experts for their risk assessments and for monitoring and evaluating the situation continuously. Currently, the installation is changing from an emergency and short-term project to a mid- and long-term monitoring solution which should provide safety for the clearance and construction works in Blatten. Additional cameras and GPS systems were installed by our team to provide an even deeper insight into the instabilities and deformations around the Kleines Nesthorn. 

How to cite: Carrel, M., Gassner, J., Wetter, J., Stitelmann, Ó., St.Pierre - Ostrander, T., and Vincent, S.: Monitoring of the "Kleines Nesthorn" and of the Birch Glacier before and during the rock avalanche in Blatten, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3801, https://doi.org/10.5194/egusphere-egu26-3801, 2026.

EGU26-5696 | Orals | NH3.5

Unsupervised Machine Learning Algorithms for Seismic Detection of Catastrophic Mass Movements 

Fabian Walter, Francois Kamper, Patrick Paitz, Matthias Meyer, Raphaël Matusiak, Michele Volpi, and Federico Amato

Catastrophic mass movements threaten mountain communities worldwide. Rockfalls, avalanches, debris flows and sediment pulses in rivers are common geomorphological processes but can destroy homes and infrastructure with little warning. Population pressure, thawing permafrost and other climatic affects will likely exacerbate this threat in the near future requiring new risk management strategies and monitoring tools.

In recent years, seismology has emerged as an efficient observational method to capture rapid mass movements and study their dynamics as well as variations in event activity. Multi-million cubic meter rock-ice avalanches like the 2025 event destroying parts of the village of Blatten, Switzerland, are often detected by national seismic networks primarily designed to monitor earthquake activity. Smaller events like rockfalls and debris flows require denser seismic networks with station spacing of a few kilometres or less. Nevertheless, their seismic signature is usually clear when seismic stations are close enough.

The straightforward detection of mass movements using seismic instrumentation has motivated new monitoring approaches. However, the challenge remains to automatically identify the seismic mass movement signature in continuous data streams given a wealth of other signals like anthropogenic noise and earthquakes, which are recorded at the same time and may mask the sought-after mass movement signals. Recent applications of machine learning algorithms have provided promising first results and allowed for mass movement detection in cases where empirical threshold-based triggering rules yield impermissible amounts of false positives.

Here we present a new approach to detect mass movements signals in continuous seismic catalogues. To tackle the challenge of algorithm transferability between sites with different seismic background noise we treat mass movement signals as anomalies given their catastrophic nature and rare occurrence. We use the isolation forest algorithm to quantify the degree of anomaly (‘anomaly score’) associated with any recorded signal. Using data from polar fjord systems, our results show that anomaly detection can efficiently reduce continuous seismic data sets to a handful of signals, which are likely related to rock avalanches and glacier break-off events. On smaller scales, anomaly scores can be processed to identify general characteristics of debris flow seismograms recorded near active torrents. The anomaly score approach thus facilitates systematically searching for large-scale mass movement seismograms in earthquake monitoring data and may be a stepping stone for flexible and transferable detection algorithms for monitoring and warning purposes.

How to cite: Walter, F., Kamper, F., Paitz, P., Meyer, M., Matusiak, R., Volpi, M., and Amato, F.: Unsupervised Machine Learning Algorithms for Seismic Detection of Catastrophic Mass Movements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5696, https://doi.org/10.5194/egusphere-egu26-5696, 2026.

In May 2025, a catastrophic debris-ice avalanche with a volume of approximately 10 million cubic meters led to the complete destruction of the village of Blatten (Valais, Switzerland). Despite tremendous destruction, and due to extensive monitoring and mitigation measures of the authorities, the residents of Blatten could be evacuated in time. The aim of this talk is to review the dynamic processes associated to the catastrophe, and the implications to the population of Blatten.

Accelerated deformation of the rock slope of Kleines Nesthorn around two weeks before the debris-ice avalanche was the first process in a cascade of events. The rock collapse was followed by 1) rock debris accumulating and loading Birch Glacier, 2) glacier collapse followed by two-phase debris-ice avalanche on 28 May 2025, 3) debris deposition as thick as 32 m onto the village of Blatten, 4) river damming in the main valley, 5) lake formation up-valley, and 6) outflow of impounded water and formation of a new river bed. The role of the inherited geology and climate on preconditioning and triggering of enhanced rock-collapse activity with a subsequent debris-ice avalanche is still debated and focus of ongoing research. Kleines Nesthorn, consisting of various metamorphic bedrock types (interlayering of jointed granitic gneisses, amphibolites, and biotite-sericite gneisses), has a complex geologic origin. The exposition and altitude of the rock flanks indicate that those bedrocks very likely were affected by the presence of permafrost. The unfavourable geology in combination with melting permafrost (and increased hydrostatic pressures) are most likely the main causes of the natural disaster. Meteorologic conditions prevailing in May 2025, such as the heavy precipitation on 28 May 2025, most likely were saturating the collapsed debris that was temporarily accumulated on Birch Glacier, resulting in a higher water content of the collapsed debris and partly explaining the runout of the event.

The village of Blatten existed since at least 1433, and through the past centuries, the population of Blatten has learnt to live with the threat of a variety of geohazards. Historic documentation shows that the two most common geohazards are snow avalanches and floodings, with recurrence intervals of 2 and 16 years for the Lötschental Valley. These records, however, lack any documentation about rock avalanches, highlighting the absence of a baseline for this type of hazard. The geohazard map of Blatten has been updated in November 2025, and its results allow to build a safe Blatten 2.0 following a well-defined roadmap, with land for building available in moderated areas, and return of residents by 2029.

The event is unprecedented for the Swiss Alps both in terms of the dynamics of collapse and its devastating impacts, and highlights that disasters can happen even on very low probabilities. Due to timely evacuation and avoided loss of life, financial support from the insurance companies and donations, and specific regulations for the case of Blatten, the mood and willingness to return to Blatten is rather high, indicating that a Blatten 2.0 has a “prosperous” future if time schedules are kept.

How to cite: Bellwald, B.: Anatomy of the Blatten rock-collapse debris-ice avalanche (28 May 2025): Insights from a local Quaternary geologist, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6599, https://doi.org/10.5194/egusphere-egu26-6599, 2026.

EGU26-6634 | Orals | NH3.5

How Rainfall and Temperature Modulate Rock-slope Stiffness: Insights from Ultrasonic and Resonance Monitoring 

Juliane Starke, Romain Rousseau, Laurent Baillet, Antoine Guillemot, and Eric Larose

Rockfalls threaten infrastructure and lives and are driven by progressive, climate-induced rock damage that weakens slopes until failure. Resonance frequency analysis can be to used to track stress evolution at the cliff (decameter) scale (1), but it lacks sensitivity to the near-surface zone where weathering initiates. We therefore combine resonance monitoring with high-frequency ultrasonic testing to resolve stress changes in this critical surface layer.

We deployed six ultrasonic transducers (two emitters and four receivers) over a few square meters on a 50-m-high south-facing limestone cliff above the Chauvet cave (SE France), while resonance frequencies were continuously recorded with a seismometer. On the one hand, repeated ultrasonic measurements provide relative sonic velocity changes as a proxy for near-surface stress changes and damage. On the other hand, resonance frequencies reflect the apparent rigidity and fracture dynamics of the entire rock column, which have been shown to track progressive damage at this site (2).

The data reveal pronounced diurnal velocity cycles driven by temperature-controlled opening and closure of micro-fractures. A major summer rainfall event caused an abrupt ~10% drop in sonic velocity, indicating a transient loss of near-surface rigidity. By constraining the surface contribution to resonance-frequency changes with the ultrasonic data and finite-element modelling, we could also show that rainfall promotes opening of the rear fracture of the cliff.

These coupled observations indicate that rainfall induces pore-pressure changes and fracture-deformation effects that temporarily reduce stiffness and accelerate sub-critical crack growth, promoting long-term slope weakening. The combined ultrasonic-seismic approach thus provides a powerful framework for quantifying climate-driven damage and improving rock-slope hazard assessment.
 

1 ) Guillemot, A., Baillet, L., Larose, E., & Bottelin, P. (2022). Changes in resonance frequency of rock columns due to thermoelastic effects on a daily scale: observations, modelling and insights to improve monitoring systems. Geophysical Journal International, 231(2), 894-906.

2 ) Guillemot, A., Audin, L., Larose, É., Baillet, L., Guéguen, P., Jaillet, S., & Delannoy, J. J. (2024). A comprehensive seismic monitoring of the pillar threatening the world cultural heritage site Chauvet‐Pont d'Arc cave, toward rock damage assessment. Earth and Space Science, 11(4), e2023EA003329.

How to cite: Starke, J., Rousseau, R., Baillet, L., Guillemot, A., and Larose, E.: How Rainfall and Temperature Modulate Rock-slope Stiffness: Insights from Ultrasonic and Resonance Monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6634, https://doi.org/10.5194/egusphere-egu26-6634, 2026.

EGU26-6995 | Orals | NH3.5

Emerging hazards in the Italian Alps under climate and environmental change 

Marta Chiarle, Erica Matta, and Guido Nigrelli

As is well known, global warming and consequent environmental changes are rapidly changing natural hazard scenarios, especially at high elevation, where the cryosphere is degrading at an accelerated rate. The increasing frequency of natural instability processes at high elevation and their change in seasonality are now well-established globally. In recent years, a growing attention has been paid to unprecedented process chains (e.g., the collapse of the Birch Glacier in 2025 in Switzerland or the huge Mount Meager event in 2010 in Canada). However, in recent years, some unusual instability processes in the Italian Alps highlighted emerging hazards that deserve further investigation. Over the three-year period from 2021 to 2023, and with intensification in 2024, the Rin da Clus torrent (Livigno, Central Italian Alps) was affected by recurring debris flow events, even in the absence of rainfall, triggered by the rapid thawing of the frontal sector of a rock glacier. In June 2024, and again in September 2024, the proglacial areas of numerous Alpine valleys in the Western Alps were devastated by an intense meteorological event, extraordinary for high mountains, which caused widespread and sometimes extreme torrential processes, initiated in Little Ice Age deposits. The most emblematic event was the collapse of the LIA frontal moraine of the Northern Grandes Murailles Glacier (Aosta Valley), which mobilized nearly 2 million cubic meters of debris. Finally, in July 2025, a portion of the debris talus on a permafrost slope in Val di Rhemes (Western Italian Alps) suddenly collapsed. Although these are isolated events and sometimes small (as in the case of the Livigno debris flows and the Val di Rhemes collapse), these phenomena draw attention to the effects of global warming on the stability of debris accumulations, which in high mountains are often steep enough to be potentially susceptible to instability. In fact, very little is known about the distribution and thermal conditions of ground ice, while the volumes of debris that can be mobilized are rarely known. These phenomena deserve careful consideration in the coming years, given the extent of debris covers in high-elevation areas, their susceptibility to instability because of slope and lack of vegetation, and the great distances that the resulting debris flows can travel.

How to cite: Chiarle, M., Matta, E., and Nigrelli, G.: Emerging hazards in the Italian Alps under climate and environmental change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6995, https://doi.org/10.5194/egusphere-egu26-6995, 2026.

EGU26-7133 | Posters on site | NH3.5

Rockfall risk mitigation in the Alps 

Guido Nigrelli, Erica Matta, Andrea Merlone, Graziano Coppa, Natali Aranda, Vincenzo Corrado, Ilaria Ballarini, Seyed Amir Afzali Fatatouei, Mamak Tootkaboni, Andrea Gramazio, and Marta Chiarle

In the alpine cryosphere, thermo-mechanical stresses due to rock temperature fluctuations, induce crack opening or widening, predisposing rock faces to failure. In the last decades, an increase in rockfalls has been documented and has been attributed to air warming. However, in-situ relationship between air and rock temperature is still little known, while a comprehensive understanding of heat transfer in rocks and their thermophysical properties are crucial to rockfall risk mitigation. This issue is being investigated in the Bessanese high-elevation experimental basin (western Italian Alps) with the following objectives: i) Use of metrologically validated Internet of Things (IoT) devices for continuous, in-situ monitoring of key parameters preconditioning rockfalls; ii) Develop an accurate heat transfer model in rock, to be used for rockfall risk mitigation in the alpine cryosphere; iii) Build a high-elevation monitoring site in rockfall-prone areas to validate the model and monitor rock temperature at different depths (10 cm, 30 cm and 50 cm); iv) Create a web portal to display the monitoring data in near-real time.

The traceability of the rock temperature measurements and the accuracy of the data are essential for the development of reliable heat transfer models in rocks. For this purpose, the six thermometers installed inside the two IoT devices at The Uja of Bessanese at different orientations, elevation and depths were previously calibrated. The calibration was made by comparing the readings of the six thermometers against a reference thermometer, in a thermal bath at different temperatures (-20 °C, -5 °C, 0 °C, 5°C, 20 °C and 40 °C). Since the sensors in the rock are not exposed to wind, direct solar radiation or other quantities of influence, the uncertainty of the instantaneous rock temperature measurements is assumed to be the same as the calibration uncertainty (0.014 °C).

A heat transfer model of rock was developed according to the following steps: i) Theoretical investigation of heat transfer in rocks, survey on simplified and detailed numerical models; ii) Set up of the COMSOL Multiphysics tool with the Heat Transfer Module; iii) Application of numerical heat transfer simulation on the monitoring site; iv) Calibration of numerical heat transfer model, establishing model reliability and accuracy, from experimental data and in-situ measurements; v) Sensitivity analyses to identify the thermal behavior of rocks with varying driving forces; vi) Rock heat transfer scenario analyses.

Main results of this work: i) Enhanced understanding of the relationships between air and rock temperature, and solar radiation at high-elevation sites; ii) Deployment of new-generation, metrologically validated IoT devices, installed in high-elevation rockfall-prone areas; iii) Development of a specific and exportable heat transfer model for metabasites; iv) Implementation of a freely accessible web portal (https://bessanese.lab3841.it). This work was carried out within the project 20223MKEMB_PE10_PRIN2022 - PNRR M4.C2.1.1 Funded by the European Union - Next Generation EU (October 2023 - February 2026).

How to cite: Nigrelli, G., Matta, E., Merlone, A., Coppa, G., Aranda, N., Corrado, V., Ballarini, I., Afzali Fatatouei, S. A., Tootkaboni, M., Gramazio, A., and Chiarle, M.: Rockfall risk mitigation in the Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7133, https://doi.org/10.5194/egusphere-egu26-7133, 2026.

EGU26-7837 | Orals | NH3.5

Rockfall data: collection methods, analysis and use for hazard and risk assessments 

Patrick Thuegaz, Davide Bertolo, Michel Stra, Francesco Agostino, and Simone Rover

On 25 December 2022, a rockfall of approximately 6,000 m³ detached from the east wall of the Mont de Nona rocky crest (Pré-Saint-Didier, Aosta Valley, NW Italy), impacting the mountain road connecting the La Thuile ski resort and the international route to France via the Piccolo San Bernardo Pass. The event triggered an emergency response by the Aosta Valley Geological Survey to support rapid, provisional risk-mitigation measures, including the construction of a rockfall embankment at the road and stabilization arrangements on the slope aimed at limiting the consequences of potential subsequent collapses.

This contribution presents an integrated, multi-sensor surveying workflow designed to document the post-event morphology and the final state of the emergency works in a steep, partly inaccessible alpine environment, and to provide an accurate topographic basis for subsequent hazard and risk evaluation. The survey combined: (i) Unmanned Aircraft System (UAS) photogrammetry supported by RTK GNSS ground control; (ii) a scanning total station acquiring high-resolution point clouds and imagery, particularly effective in areas with limited aerial visibility; and (iii) a high-performance GNSS receiver to precisely determine the occupied scanning-station positions within a global reference system, enabling rigorous georeferencing of the terrestrial dataset through a traditional traverse approach.

Post-processing integrated terrestrial and aerial point clouds into a single 3D dataset and applied classification tools to separate vegetation and bare ground, producing a Digital Elevation Model (DEM) of the site. The DEM was subsequently used to extract targeted 2D cross-sections along the slope–road system to support verification of the embankment geometry and to frame scenario-based assessments of residual rockfall hazard.

The case study demonstrates how complementary survey technologies can be effectively combined to deliver rapid, accurate, and operationally robust terrain models for alpine mass-movement emergencies. UAS mapping provides efficient coverage of large and impervious areas, while scanning total station data ensures high spatial resolution and completeness where aerial viewpoints are limited. GNSS-based georeferencing ensures that products are immediately interoperable with regional geodata and suitable for follow-up analyses, supporting decision-making in time-critical risk management contexts.

How to cite: Thuegaz, P., Bertolo, D., Stra, M., Agostino, F., and Rover, S.: Rockfall data: collection methods, analysis and use for hazard and risk assessments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7837, https://doi.org/10.5194/egusphere-egu26-7837, 2026.

EGU26-9045 | ECS | Orals | NH3.5

Dynamics and precursors of the 2025 Blatten rock–ice avalanche: Integrating seismic analysis, granular flow simulations, and field observations 

Jiahui Kang, Antonie Lucas, Anne Mangeney, Johan Gaume, Kate Allstadt, Clément Hibert, Liam Toney, Hervé Vicari, Michael Dietze, Mylène Jacquemart, Marc Peruzzetto, Lars Blatny, Michael Kyburz, Joachim Rimpot, Daniel Farinotti, and Fabian Walter

Cascading slope failures in high mountain environments are observed with increasing frequency as glaciers retreat and slope stability is impacted by warmer conditions. On 28 May 2025, a large rock-ice avalanche (~9.3x106 m3) originating from Birch Glacier, Switzerland, destroyed parts of the village of Blatten, and provided a rare, well-documented case of a rapid, highly mobile mass movement.

We combine seismic observations, geomorphological mapping, grain size and permeability measurements, and granular flow modelling to reconstruct the evolution of this event, from precursory instabilities to the main collapse. Seismic data scanned with machine learning algorithms reveal a two-week period of increasing rockfall and small glacier failures preceding the main collapse. The main collapse was reconstructed using force history inversion of low-frequency seismic signals from Switzerland’s national seismic network. Numerical simulations constrained by both seismic data and observed deposit extents indicate that an exceptionally low effective basal friction was required to reproduce the observed deposit extent and force history. This and the field observations of low-permeability deposit materials indicate that frictional weakening contributed to the unexpectedly high mobility of the main event.

Our results highlight the value of integrating seismic monitoring with field and modelling approaches to constrain the dynamics of complex rock-ice avalanches. The Blatten event illustrates how large alpine slope failures can transition into highly mobile flows. Our study provides one of the first detailed reconstructions of this hazard cascade, including precursory failure activity, and the dynamics and frictional characteristics of the main event. The frictional weakening inferred here provides a much-needed mechanistic basis for predicting runout and deposit geometry in large debris avalanches.

How to cite: Kang, J., Lucas, A., Mangeney, A., Gaume, J., Allstadt, K., Hibert, C., Toney, L., Vicari, H., Dietze, M., Jacquemart, M., Peruzzetto, M., Blatny, L., Kyburz, M., Rimpot, J., Farinotti, D., and Walter, F.: Dynamics and precursors of the 2025 Blatten rock–ice avalanche: Integrating seismic analysis, granular flow simulations, and field observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9045, https://doi.org/10.5194/egusphere-egu26-9045, 2026.

Many alpine valley infills could be hiding deposits of large rockfall events that have occurred since the end of the last glaciation. This could lead to incomplete bergsturz inventories and a skewed risk assessment. In the Reintal valley near Mount Zugspitze in the Wetterstein Mountains (Germany), two bergsturz events are known to have occurred, and a third, covered event, is highly likely. The two known events are the Blaue-Gumpe bergsturz with a volume of 1.5 million m3 and an age of approximately 200 years and the Steingerümpel bergsturz with a volume of 2.5 million m3 and an age of 400-600 years. For the covered third event an age of approximately 1,000 years is estimated. However, no other bergsturz or large rockfall events are known. Two to three bergsturz events have occurred in the Reintal valley within approximately 800 years, but the valley has been ice-free for approximately 12,000 years. Several bergsturz events are known to have occurred in neighboring regions over the last 4,000 years. Therefore we hypothesize that further bergsturz or large rockfall events may have occurred during the Holocene and late Pleistocene and are sediment covered. Here we present evidence derived from electrical resistivity tomography (ERT), supported by morphological findings, for two potential further bergsturz or large rockfall events hidden in the valley infill. In a 4.6 km long ERT-profile along the valley floor, two surface anomalies with increased and locally highly variable resistivity can be identified, which are similar in their characteristics to the two known bergsturz events. One of these areas can be linked to a potential detachment scarp above. There, the anomaly in the ERT profile also corresponds to a section along the Partnach River where the gradient is significantly increased and river meanders are more pronounced than in the rest of the river course. The second area is more pronounced in the ERT-Profile but doesn’t show any obvious morphological features. Based on these results, it is likely that two previously unknown large rockfall events are hidden in the valley infill. If these new potential large rockfall events are confirmed, rock slope failure rates in the well-studied Reintal valley, and thus possibly in the entire Wetterstein Mountains and adjacent mountain ranges, could increase, which has significant implications for hazard reassessment.

How to cite: Hofner, M., Lehmann, P., and Krautblatter, M.: Presenting Evidence of previously unknown Bergsturz Events, contributing to Long Term Rock Slope Failure Rates in an Alpine Valley (Reintal, Wetterstein Mountains, Germany), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9473, https://doi.org/10.5194/egusphere-egu26-9473, 2026.

EGU26-9717 | ECS | Orals | NH3.5

Multiple comparisons of point clouds acquired by a permanent LiDAR (PLS) to improve the reliability of a rockfall event catalogue 

Sara Susini, Clara Lévy, Marie-Aurélie Chanut, Thomas J. B. Dewez, and David Amitrano

The ANR C2R-IA project (www.anrc2ria.fr) aims to develop reliable decision-support tools for the dynamic management of rockfall hazard. Its goal is to understand how meteorological forcing influences rockfall occurrence and to anticipate temporary increases in hazard in order to implement risk reduction measures. To this end, a predictive model of rockfall occurrence as a function of meteorological conditions is being developed using artificial intelligence tools (neural network training), which requires a comprehensive and well-labelled dataset. Several monitoring instruments have been deployed at the Saint-Eynard site (Grenoble, France). Among them, a permanent LiDAR scanner (PLS) acquires point clouds continuously, with one acquisition per hour, providing high temporal resolution representative of what could be used for operational monitoring or crisis management. An automated data-processing workflow has been developed in Python. It is based on a pairwise comparison of the clouds (Manceau et al., 2025) and includes the alignment of successive point clouds, filtering of points outside the cliff area, change detection using M3C2 distances computation, clustering with DBSCAN, and volume quantification of rockfalls using alphashapes. This well-structured processing has significantly reduced the detection threshold, identifying relief change of only 10 cm deep (compared to 40 cm previously; Le Roy et al, 2020) and 10 liters in volume, while the scanner is located approximately 1 km from the cliff. Depending on acquisition quality, the effective temporal resolution of detected rockfall events may range from one hour to several days. Combining relief-change detections with simultaneously deployed seismic monitoring should further refine event timing. The completeness of the event catalogue has therefore improved, increasing from fewer than 10 detected rockfalls per month to around 30. However, some false positives remain, mainly related to recurring artifacts despite preprocessing. To mitigate these errors, the previous pairwise comparison of the clouds has been refined to a multiple point-cloud comparison strategy, enabling the tracking of the temporal persistence of changes. This allows distinguishing changes corresponding to real rockfalls, which persist over time, from transient artifacts. This improvement leads to a more reliable and complete rockfall event database. It includes block shape ratios, identified failure mechanisms, and free-fall heights under overhanging sections, providing a suitable basis for future fusion with seismic data.

Manceau, L., Chanut, M.-A., Levy, C., Dewez, T., and Amitrano, D.: Enhancing Rockfall Detection Using Permanent LiDAR Scanner (PLS) Data and Automated Workflows at St. Eynard Cliff (Grenoble, France), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6312, https://doi.org/10.5194/egusphere-egu25-6312

Le Roy, G., Helmstetter, A., Amitrano, D., Guyoton, F., & Le Roux-Mallouf, R. (2019). Seismic analysis of the detachment and impact phases of a rockfall and application for estimating rockfall volume and free-fall height. Journal of Geophysical Research: Earth Surface, 124, 2602-2622. https://doi.org/10.1029/2019JF004999

How to cite: Susini, S., Lévy, C., Chanut, M.-A., Dewez, T. J. B., and Amitrano, D.: Multiple comparisons of point clouds acquired by a permanent LiDAR (PLS) to improve the reliability of a rockfall event catalogue, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9717, https://doi.org/10.5194/egusphere-egu26-9717, 2026.

EGU26-9865 | Posters on site | NH3.5

Influence of folds and fold-related faults on slope stability 

Alexandra Schagerl and Alexander Preh

Geological structures such as folds have a significant influence on the behaviour and stability of slopes, foundations and tunnels in hard rock (Badger 2002). Although the importance of structural geology for geotechnical buildings has long been recognized, in practice it is often not consistently taken into account in all project phases.

In geotechnical models, discontinuities such as joints, schistosity and bedding planes, as well as faults, are usually represented as flat surfaces. Nevertheless, this simplification only corresponds to reality to a limited extent: discontinuities are often corrugated, and the location of folds and fold-related joints can significantly influence the stability of slopes. However, more recent approaches also integrate fold geometries (Fereshtenejad, Afshari et al. 2016, Erharter 2024) to realistically capture their influence on slope stability.

Variations in the position of folds can promote different failure mechanisms, while certain fold orientations can have a stabilizing effect.

Against this background, the following key question arises: To what extent is it permissible to simplify surfaces to flat surfaces, and how can folds be realistically represented in numerical models?

To determine the discontinuity system (fracture network) and the relevant structural parameters, the rock outcrops to be investigated are surveyed using UAV flights. The photogrammetric images obtained are processed using special software such as Agisoft Metashape, and high-resolution textured terrain models are derived from them. These serve as the basis for stereographic analyses, geotechnical evaluations and the calculation of discrete fracture networks.

In addition, the effects of the spatial location of the fold and joint systems on the stability of the surveyed rock surfaces are investigated using the discrete element method (Particle Flow Code; Itasca). The discrete fracture networks derived from UAV photogrammetry are integrated into the models and the spatial location of the slope (exposed rock surface) is varied. In this way, the influence of the fold position on the stability of the rock faces under investigation is systematically examined.

The results should reveal systematic relationships between fold geometry, joint distribution and slope stability, improve understanding of structurally induced instabilities and support the further development of geotechnical assessment methods in rock mechanics.

How to cite: Schagerl, A. and Preh, A.: Influence of folds and fold-related faults on slope stability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9865, https://doi.org/10.5194/egusphere-egu26-9865, 2026.

EGU26-10264 | ECS | Orals | NH3.5

Automated seismic monitoring of mass movements in the Mont-Blanc massif  

Jakub Kokowski, Agnès Helmstetter, Eric Larose, Ludovic Ravanel, and Xavier Cailhol

Mass movements in the Mont-Blanc massif (French Alps) are traditionally monitored by a network of human observers (AlpRisk and ObsAlp networks in the past and Regard d’Altitude currently) and annual LiDAR campaigns for some areas. These observations provide accurate locations and estimates of event size. However, those approaches have several limitations: observations are biased toward areas frequently visited by people and are potentially incomplete in remote regions. In addition, temporal accuracy is frequently poor (except during peak periods for mountaineers), as many observations are based on debris deposits rather than on the events themselves.

Seismic monitoring using permanent seismic stations installed in the area offers a promising complementary solution to these limitations. Rapid mass movements such as serac collapses and rockfalls generate particular seismic signals, providing excellent temporal resolution and continuous coverage, including in areas that are rarely observed directly. Their seismic signatures differ significantly from those of earthquakes, requiring dedicated methods for event localization and size estimation.

Based on field observations of mass movements and the Sismalp seismic event catalog, we compiled a reference catalog currently consisting of 107 seismic events associated with 91 field observations, including volume estimates for 55 events. This catalog was used to fine-tune and evaluate automated algorithms for the localization and size estimation of mass movements using seismic data.

Mass movement localization is performed using a combination of an amplitude decay method and the BackTrackBB algorithm based on signal coherence. We achieved a median location accuracy of 1.6 km and observed a significant improvement in localization accuracy with increased seismic station coverage. Event size was estimated using a simple linear model based on seismic energy, resulting in a median relative error of approximately 70 %.

Our results show that automated seismic monitoring of mass movements can be successfully applied in remote high-mountain environments. The performance of our method can be further improved by increasing the number of seismic stations and by improving data processing techniques.

How to cite: Kokowski, J., Helmstetter, A., Larose, E., Ravanel, L., and Cailhol, X.: Automated seismic monitoring of mass movements in the Mont-Blanc massif , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10264, https://doi.org/10.5194/egusphere-egu26-10264, 2026.

EGU26-10355 | Orals | NH3.5

Calibration and validation of rockfall modelling along a railway section in an mountain area in Central Italy 

Francesca Ardizzone, Mauro Rossi, and Michele Santangelo

Rockfalls represent a substantial threat to railway routes, due to their rapidity, destructive potential and high probability of occurrence on steep topographies. Approaches for the assessment of rockfall susceptibility range from statistical methods, for modeling large areas, to deterministic ones, for application in local analyses. A common requirement is the need to locate the source areas, often found uphill on cliffs, and the subsequent assessment of the runout areas of rockfalls stemming from such areas. Modelling rockfall phenomena is complex and requires various inputs, including: accurate location of the source areas,  geomorphological and  geological setting, and other geo-environmental factors.

We present an application conducted along the Rocca San Zenone - Giuncano Scalo railway line, in a study area (26 km2) in Central Italy,  where rockfall are abundant. The activity consisted in creating rockfall trajectory maps, in geotiff format, starting from possible source areas, and in classifying and validating the maps. The following software was used to create the trajectory map: i) rockyfor3D (https://www.ecorisq.org/ecorisq-tools); and ii) STONE (Guzzetti et al., 2002). The classification and validation phase was carried out using the R RF-Tools software (Rossi, 2023). Methodology for the Creation of Landslide Susceptibility Maps to produce rockfall susceptibility zoning, considering three scenarios: i) plausible scenario, ii) best case scenario; and iii) worst case scenario.

The rockfall modeling procedure was developed as part of a national project dedicated to the preparation of an operational methodology for assessing landslide susceptibility along the entire Italian railway network.

How to cite: Ardizzone, F., Rossi, M., and Santangelo, M.: Calibration and validation of rockfall modelling along a railway section in an mountain area in Central Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10355, https://doi.org/10.5194/egusphere-egu26-10355, 2026.

EGU26-10578 | ECS | Posters on site | NH3.5

Building an Open Collection of Mass Movements and Their Environmental Drivers in Austria 

Jakob Klotz and Willemijn van Kooten

Global warming and its effects on precipitation and temperature patterns affect the frequency and magnitude of mass movements, particularly the occurrence of rockfalls, debris flows and landslides in high-elevation regions. The expected change in mass movement activity makes a systematic hazard documentation and analysis of possible drivers particularly urgent. An important step toward risk assessment in prone areas is the development of comprehensive mass movement inventories that record time, location, process type and various attributes of past events and ongoing processes. Yet, despite hosting a substantial share of the Alps and having more than 60% mountainous territory, Austria lacks a complete and open-access inventory suitable for analyzing the relationship between mass movements and their drivers. Similarly, high quality data sets of environmental attributes (e.g., precipitation, soil moisture, lithology and topography) exist, but are currently not collected within a single database and linked with mass movement events in the Austrian Alps.

We introduce the open Collection of Mass Movements in Austria (oCoMMA), an expandable harmonized framework provided as FAIR-aligned PostGIS database of mass movement events in Austria, compiling openly available records from peer-reviewed studies and national authorities. Reproducible workflows for type standardization and event de-duplication support consistency and transparency. The continuous integration of updated data sets and transparent documentation facilitates interoperability for researchers and practitioners. Through statistical analysis of mass movement drivers, we aim to reveal new insights into triggers of rockfalls, debris flows and landslides. The objective of oCoMMA is to provide a new open-access foundation for evidence-based risk management in Austria’s mountain regions and to accelerate further research to protect communities and infrastructure.

How to cite: Klotz, J. and van Kooten, W.: Building an Open Collection of Mass Movements and Their Environmental Drivers in Austria, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10578, https://doi.org/10.5194/egusphere-egu26-10578, 2026.

The crack propagation and coalescence mode play an important role in the step-path failure mechanism of rock slope. This study uses the discrete element method (DEM) to simulate the modes of crack coalescence in rock. Initially, coalescence modes between two pre-existing cracks with different geometries (rock bridge angle) and confining stress under biaxial compression were performed. Several modes and their dependence on conditions were observed. During the tests, wing cracks and secondary cracks have been identified, which manifested as tensile and shear cracks in a plane coplanar with the pre-existing cracks. Particularly, the secondary cracks can be either shear or tensile cracks depending on its geometries and confining stress, and they progressively transition from tensile to shear with the increase of confining stress. The wing cracks always occurred under a low confining stress biaxial compression and almost disappeared under a high confining stress. In addition, confining stress can influence on the crack coalescence modes dramatically. Therefore, a set of extended coalescence modes has been proposed to analyze interactions among multiple flaws, demonstrating that the crack coalescence preferentially occurs between the pair of flaws associated with low coalescence stress. Finally, a rock slope case was conducted to elucidate the step-path failure mechanism. The results show that joint coalescence initiates at the slope toe and subsequently propagates upward. Distinct coalescence modes, governed by the local stress conditions within the slope, control the development and irregularity of the failure surface.

How to cite: Zhu, L.: Study of the step-path failure mechanism of rock slope based on crack coalescence modes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11034, https://doi.org/10.5194/egusphere-egu26-11034, 2026.

EGU26-11285 | ECS | Posters on site | NH3.5

Controls on rockfall hazard and risk metrics at critical spots of access roads to Yosemite Valley (California, USA) 

Rebecca Bruschetta, Federico Agliardi, Paolo Frattini, Greg M. Stock, Filippo Giorgi Spreafico Del Corno, and Brian D. Collins

Yosemite National Park (California, USA) is characterized by high-relief granitic cliffs shaped by complex geological processes and forming iconic geomorphological features, including exfoliating granite and a steep glacially carved landscape. This setting results in frequent, often intense rockfall activity that poses a significant threat to humans, property and utilities along the road network accessing Yosemite Valley. Quantitative assessment of rockfall risk along these roads (El Portal, Big Oak Flat and Wawona) relies on synthesized metrics that integrate both hazard and exposure of elements at risk.

Rockfall hazard depends on release mechanisms and magnitude–frequency relationships. Slope topography and materials (e.g. fine vs coarse talus, shallow soil covering) also play a critical role influencing energy dissipation, trajectory dispersion or convergence. These factors ultimately determine the frequency, energy, and fly height of rockfalls reaching road segments. Exposure is mainly governed by traffic characteristics such as vehicle density, speed, and occupancy. Comparable risk values across different sites may be a result of different combinations of hazard and exposure factors, underscoring the need for site-specific mitigation strategies.

We assessed rockfall hazard and risk along Yosemite Valley access roads using high-resolution (1 m) 3D rockfall runout simulations performed with the Hy–STONE simulator combined with a historical rockfall inventory (1857–2023) and traffic data provided by the National Park Service. Hazard was quantified using a modified Rockfall Hazard Vector (RHV) method incorporating block kinetic energy, fly height, and a normalized annual frequency derived from both onset frequencies from inventory analyses and propagation frequencies from runout modeling. Although originally conceived as a susceptibility index, the modified RHV provides an effective proxy for quantitative hazard. Rockfall risk was computed by integrating hazard with exposure and vulnerability parameters, including vehicle speed, size, and traffic volumes. The road network was discretized into 10 m segments for each travel lane (inbound and outbound from Yosemite Valley), and risk was evaluated for different rockfall volume scenarios (0.01–100 m³) while accounting for model uncertainties. For each segment, the annual probability of loss of life (E(LOL)) was estimated under different traffic conditions.

The results identify several critical road sections where the distribution and magnitude of elevated risk arise from distinct combinations of hazard and exposure contributions. For example, in the Parkline sector, high risk conditions are dominated by high hazard concentrated within a narrow corridor and related to exfoliation sheet failures from a steep cliff directly above the road with risk further amplified by congested traffic patterns. At Windy Point, comparable risk levels are associated with lower hazard levels in an area with multiple small, structurally controlled sources, but with higher exposure to widespread rockfall trajectories and adverse traffic conditions. Conversely, at the junction between Big Oak Flat and El Portal Roads, high risk is dominated by exposure linked to traffic flow convergence despite moderate hazard levels.
These findings highlight the importance of disentangling the individual factors contributing to quantified risk metrics to design targeted and effective mitigation strategies for rockfall risk along park access roads and more widely to mountain roads.

How to cite: Bruschetta, R., Agliardi, F., Frattini, P., Stock, G. M., Giorgi Spreafico Del Corno, F., and Collins, B. D.: Controls on rockfall hazard and risk metrics at critical spots of access roads to Yosemite Valley (California, USA), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11285, https://doi.org/10.5194/egusphere-egu26-11285, 2026.

EGU26-12337 | ECS | Orals | NH3.5

Physics-Informed Seismic Inference of Rockfall Sources and Motion Regimes 

Shuaixing Yan, Zhuowei Li, and Dongpo Wang

Rockfalls radiate complex seismic signals that encode both evolving source dynamics and path-dependent interactions, yet these signals are rarely exploited to support real-time trajectory inference within a unified framework.Here we develop a physics-constrained framework that integrates deep learning with forward motion modeling to jointly infer rockfall source location and motion mode from multi-station seismic observations, and to translate these inferences into early trajectory prediction.A spatiotemporal network combining temporal convolution and graph convolution exploits inter-station waveform variability to estimate three-dimensional source locations and discriminate motion regimes in near real time.Field experiments in China and the French Alps demonstrate meter-scale localization accuracy and enable early estimates of subsequent impact points before terminal deposition, providing actionable lead time for dynamic hazard response.Guided by rockfall source–path mechanisms, we further introduce spatial information as a physically meaningful proxy for propagation effects, which substantially improves motion-mode discrimination and yields spectrally coherent attention patterns consistent with observed impact and rolling processes.Finally, we show that localization accuracy is jointly controlled by dataset size and spatial scale, revealing that site-scale effects can outweigh gains from simply increasing sample numbers.Together, these results demonstrate that embedding physical cognition into deep learning enables seismic wavefields to be translated into real-time, interpretable constraints on rockfall dynamics, outlining a pathway toward physics-informed monitoring of gravity-driven hazards.

How to cite: Yan, S., Li, Z., and Wang, D.: Physics-Informed Seismic Inference of Rockfall Sources and Motion Regimes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12337, https://doi.org/10.5194/egusphere-egu26-12337, 2026.

EGU26-12511 | ECS | Orals | NH3.5

Towards statistical alarm threshold determination for alpine rock fall monitoring systems 

Johannes Leinauer, Maike Offer, Ingo Hartmeyer, Matthias Hofner, and Michael Krautblatter

Alpine rock slope failures are frequent hazardous events. To reduce risk, unstable rock sections are increasingly monitored, e.g. with automatic displacement and tilt meters or high-resolution remote techniques. However, effective mitigation actions require the triggering of meaningful alarms. Currently, these alarm thresholds are often set manually based on expert knowledge, which may create too conservative or insufficiently sensitive thresholds that are not well enough adapted to changing conditions over time. Instead, we hypothesise that dynamically updated thresholds based on statistical analyses of continuous observations can provide a more robust, comprehensible, and performant approach to early warning.

Here, we present an approach to determine alarm thresholds for automatic monitoring devices based on statistical analyses of past observation data of two high-alpine sites. We analyse multiple years of automatic measurements gathered from high-frequency real-time monitoring systems. At the Hochvogel summit (DE/AT; 2,592 m a.s.l.), we monitor a 200,000 to 600,000 m³ complex rock slope instability with 12 sensors since 2019 and no major rock fall event yet. The second site at the Kitzsteinhorn north flank (AT; 3,029 m a.s.l), includes 6 sensors and a 600 m³ rockslide failure in August 2025 that has been recorded by the displacement sensors. Preliminary results show that this approach is able to reduce the frequency of false alarms over time and can detect critical accelerations earlier than fixed manual thresholds.

We anticipate that this statistical analysis of multiple years of observations including failure and non-failure events can guide decision-makers and monitoring system operators on how to set initial reasonable alarm thresholds and how the thresholds can be adjusted over months and years of system operation for an early detection of hazardous accelerations.

How to cite: Leinauer, J., Offer, M., Hartmeyer, I., Hofner, M., and Krautblatter, M.: Towards statistical alarm threshold determination for alpine rock fall monitoring systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12511, https://doi.org/10.5194/egusphere-egu26-12511, 2026.

EGU26-13461 | ECS | Posters on site | NH3.5

Investigation and multi-scale monitoring of rockfall processes: Setup and preliminary results of the in-situ rock-slope laboratory at the Stubai Glacier, Tyrol (Austria) 

Hannah Andlinger, Christine Fey, Herbert Formayer, and Christian Zangerl

Rockfalls are widespread processes in alpine landscapes, shaping landscape evolution while posing significant hazards to people and infrastructure. Rapid global warming leads to accelerated glacier retreat and permafrost degradation which alter the factors that predispose, trigger and control rock slope behavior, making it difficult to apply past experiences and knowledge to present-day conditions. In this context, a process-based understanding of geological, geomechanical and meteorological precursor factors that lead to slope instabilities is crucial. Specifically, continuous, multi-scale and multi-sensor observations are essential to understand predisposing factors and to characterize acceleration phases for estimating the timing of failures.

To address this challenge, we have established the in-situ rock-slope laboratory at the Schaufelspitze, Stubai Glacier (Tyrol, Austria), where rock slope instabilities at different scales are investigated using an integrated, multi-sensor monitoring setup. This location at an elevation between 2880 and 3332 m is an ideal test setting, combining recent rock slope activity with rapid deglaciation, evolving thermal regimes and changing meteorological intensities. The established and ongoing monitoring network combines in-situ temperature sensors and crackmeters with remote sensing techniques, including terrestrial laser scanning (TLS), unmanned aerial vehicle (UAV)-based thermal and photogrammetric surveys, ground-based interferometric synthetic aperture radar (GB-InSAR), time-lapse webcam photomonitoring , and meteorological data from nearby stations.

Preliminary results show that the designed remote sensing methods, complemented by in-situ sensors, allow to observe rock slope deformations across a wide range of both spatial and temporal scales. In this study, GB-InSAR shows more applicability to identify short-term accelerations and heterogeneous patterns that are difficult to capture with episodic surveys (e.g., with TLS or UAV). In addition, the use of thermal imaging adds information indicating surface temperature anomalies related to increased rock mass fracturing and loosening as well as water pathways and springs. In-situ temperature sensors capture spatial and temporal temperature variations, enabling the identification of potential rockfall activation areas.

The rock-slope laboratory aims therefore to establish a long-term record of acceleration and deformation phases of different processes and scales, as well as to identify predisposing and triggering mechanisms of specific conditions knowing the exact event timing. Particularly by integrating multiple sensors, it aims to identify robust, transferable triggers and possibly derive practical thresholds to support future early warning systems in high alpine environments. By combining remote sensing and in-situ data, this framework provides insights on slope processes in response to hydro-meteorological factors, which would be difficult to resolve using individual techniques.

Outputs will include: (i) the identification of different scaled rockfall processes in a high alpine setting; (ii) the characterization of rock slope instability drivers, acceleration phases and failure, and (iii) validated workflows for sensor setups and combinations, change detection and photomonitoring.

How to cite: Andlinger, H., Fey, C., Formayer, H., and Zangerl, C.: Investigation and multi-scale monitoring of rockfall processes: Setup and preliminary results of the in-situ rock-slope laboratory at the Stubai Glacier, Tyrol (Austria), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13461, https://doi.org/10.5194/egusphere-egu26-13461, 2026.

EGU26-14112 | ECS | Posters on site | NH3.5

Microseismic signature of the internal deformation in the Åknes rockslide (Norway): Four years of downhole observations 

Peter Niemz, Nadège Langet, and Volker Oye

Norway’s rugged western coastline is dominated by steep mountain slopes rooted within fjords. Mass movements on these slopes pose major hazards due to the potential for triggering massive tsunamis in the narrow fjords. However, our understanding of the internal triggering processes and potential precursory signals is still limited. We use the Åknes rockslide in western Norway as a natural laboratory to study the seismic footprint of the internal deformation in a slow-moving unstable rockslide (1-3 cm/yr). The Åknes rockslide is one of the most thoroughly instrumented rockslides in the world. We analyze four years (2021-2025) of microseismic data from an 8-level three-component borehole geophone string (15-50 m below ground level) intersecting at least one of the alleged sliding planes of the rockslide. The detected microseismicity shows bursts of highly similar events located close to the well (meters to a few tens of meters) with activity varying with depth. By connecting our long-term in-situ observations with comprehensive datasets of groundwater levels and deformation measurements from other boreholes within the rockslide, we shed light on the observed microseismic processes and their driving forces in the vicinity of the monitoring well. In addition to improved process understanding, our work aims to contribute to the development of robust, physics-informed strategies for early warning of sudden rock mass mobilization.

How to cite: Niemz, P., Langet, N., and Oye, V.: Microseismic signature of the internal deformation in the Åknes rockslide (Norway): Four years of downhole observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14112, https://doi.org/10.5194/egusphere-egu26-14112, 2026.

Effective rockfall protection design requires accurate estimation of impact forces and movement trajectories. Current practices predominantly depend on numerical simulations or Optical techniques to inversely derive kinematic parameters. However, these optical methods are limited by occlusion, perspective distortion, and the inability to capture high-frequency internal impact dynamics. While previous studies have utilized MEMS-embedded Smart Rocks to monitor internal states and reconstruct 4D trajectories, existing devices are often constrained by hardware specifications. Insufficient sampling rates (typically below 1 kHz) fail to capture millisecond-level impact peaks, resulting in signal aliasing, while sensor saturation during high-intensity collisions leads to attitude divergence during attitude estimation.

To address these limitations, this study presents "Smart Rock Node (SaRoN)", a smart sensing module embedded in a 30 cm reinforced concrete shell. This design ensures the probe's mechanical properties, specifically density and coefficient of restitution, closely mimic natural boulders, ensuring the kinetic data reflects realistic rockfall behavior. It features a 1600 Hz sampling rate to prevent peak clipping and integrates a dual-sensor architecture, combining a high-G accelerometer (±200 g) and a precision IMU (±16 g, ±4000 dps), to ensure a wide dynamic range. The hardware employs a centrally-mounted computing unit with a ring buffer to eliminate data writing latency. On the algorithmic level, we introduce an adaptive impact-gating mechanism. This algorithm dynamically decouples the gravity vector dependence during collision moments, automatically pausing acceleration correction to mitigate filter divergence. This is complemented by a 1 ms timestamp synchronization protocol, ensuring precise temporal alignment for robust multi-sensor fusion. Reliability and accuracy were validated through pendulum, free-fall, and shaking table experiments, confirming trajectory consistency, structural robustness, and acceleration fidelity. Notably, Power Spectral Density (PSD) and Magnitude Squared Coherence (MSC) analyses were employed to calibrate the frequency response and confirm the credibility of event frequencies across operational bands. For field validation, a full-scale experiment is planned for the Jinheng Park slope in Taroko Gorge. The setup integrates SaRoN with a multi-modal observation network: SmartSolo and geophones to pinpoint impact locations via seismic signals, while Distributed Acoustic Sensing (DAS) installed on rockfall sheds monitors structural stress waves to assess impact intensity, UAV combined with ArUco markers serves as ground truth for validating attitude and trajectory verification.

Results demonstrate that the SaRoN system mitigates signal saturation during high-intensity impacts and shows good agreement with ground truths, highlighting its potential for capturing complex rockfall dynamics, providing high-fidelity kinematic data essential for advancing rockfall protection engineering.

Keywords: Trajectory Reconstruction, Smart Rock Node (SaRoN), Rockfall Impact force, Distributed Acoustic Sensing (DAS).

How to cite: Tseng, K.-C., Chao, W.-A., and Ou, T.-H.: Development of a High-Temporal-Resolution Smart Rock System Integrating Multi-Modal Observations: Trajectory Reconstruction and Impact Inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15178, https://doi.org/10.5194/egusphere-egu26-15178, 2026.

EGU26-16085 | Orals | NH3.5

Three-dimensional rockfall modeling in GRASS GIS with r.stone 

Massimiliano Alvioli, Fausto Guzzetti, and Andrea Antonello

We present an open-source version of the software STONE [1] for the three-dimensional simulation of rockfall trajectories. The software implements a lumped mass kinematic model that simulates trajectories in a spatially distributed manner, in areas of up to thousands of square kilometers, starting from topographic (digital terrain model, DTM) and ancillary data easily manageable in GRASS GIS [2,3].

The rockfall phenomena that can be described with the STONE model are those involving the fall of individual blocks, which do not interact during their motion with other moving blocks/boulders, and whose trajectory can be described by a combination of parabola sections (free fall), bouncing on the ground and rolling.

In addition to a DTM, minimal data required for running the r.stone module are: a raster map of the numerical coefficient of friction, relevant for the rock rolling phase, two maps of numerical coefficients of normal and tangential restitution, which control the loss of kinetic energy at each bounce, and a raster map defining the initiation points of trajectories (sources). The latter is the most distinguishing input of the software, as the simulated motion of the falling block starts at these user-defined points of the topography.

In this contribution, in addition to presenting the new software, we discuss methods to obtain the location of rockfall sources on large areas, based on different strategies. These strategies mostly involve using maps of known source locations, either observed in the field or inferred from expert mapping, and generalizing them to other possible source locations with statistical and/or machine learning methods, under the common denominator of using information from a DTM as a starting point. In the definition of rockfall sources, specific triggering events can be taken into account, such as earthquakes [4,5] or intense rainfall events [6].

The main output of the model is the count of trajectories crossing each DTM grid cell, for given source locations and number of simulated trajectories. The output can be ascribed a probabilistic meaning, to obtain a physically-based susceptibility map for rockfalls. The absolute values in the raster output can be classified according to different criteria, mostly depending on the specific target relevant to the study, typically transport corridors (railways [3], roads [7,8]), buildings, and other urban infrastructure [9].

The software manual is available on the GRASS GIS addons repository [10].

[1] F. Guzzetti et al., Computers & Geosciences 28, 1079-1093. https://doi.org/10.1016/S0098-3004(02)00025-0

[2] F. Guzzetti et al., Environmental Management 34, 191–208. https://doi.org/10.1007/ s00267-003-0021-6

[3] M. Alvioli et al., Rockfall susceptibility and network–ranked susceptibility along the Italian railway. Engineering Geology 293, 106301. https://doi.org/10.1016/j.enggeo.2021.106301

[4] M. Alvioli et al., Landslides 21(1) 1-16 (2024). https://doi.org/10.1007/s10346-023-02127-2

[5] M. Alvioli et al., Geomorphology, 429, 108652 (2023). https://doi.org/10.1016/j.geomorph.2023.108652

[6] M. Alvioli & M. Melillo (in preparation)

[7] B. Pokharel et al., Bulletin of Engineering Geology and the Environment 82, 183. https://doi.org/10.1007/s10064-023-03174-8.

[8] M. Santangelo et al., Nat. Hazards Earth Syst. Sci. 19, 325-335 (2019). https://doi.org/10.5194/nhess-19-325-2019

[9] M. Santangelo et al., Journal of Maps 17, 124 (2021). https://doi.org/10.1080/17445647.2020.1746699

[10] https://grass.osgeo.org/grass-stable/manuals/addons/r.stone.html

How to cite: Alvioli, M., Guzzetti, F., and Antonello, A.: Three-dimensional rockfall modeling in GRASS GIS with r.stone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16085, https://doi.org/10.5194/egusphere-egu26-16085, 2026.

Rockfalls are fast-moving, high-energy events that can significantly threaten lives and property, especially in residential areas and near road cuttings. The study area stand along the 350-meters section of the flanks of a main motorway connecting Birecik and Halfet districts of Şanlıurfa (SE Türkiye) where a rockfall happened in 2019. The rockfall area has considerable traffic and is located near the historic Silk Road and breeding sites of the endangered Waldrapp bird, making it both ecologically and culturally significant.

After the 2019 rockfall event, UAV-based surveys were conducted to generate a high-resolution 3D digital terrain model of the slopes. Subsequently, studies covered an application of the Rockfall Hazard Rating System (RHRZ) to evaluate the risk. Studies also include kinematic analysis, numerical analyses and rockfall simulations. In order to determine the rock mass parameters of the Miocene-aged clayey limestones that compose the slopes, discontinuity measurements were conducted as part of engineering geological studies. Additionally, laboratory tests were conducted on block samples collected from the field. The geomechanical measurements revealed that the rock material's unit weight varied between 18.1 and 21.2 kN/m³ and its uniaxial compressive strength varied between 9 and 15 MPa.

The rockfall risk for the stable sections of the slope was found to be 79 according to RHRZ, indicating high risk. All three forms of failure mechanisms; planar, wedge-type, and toppling-type were determined to have the potential to occur after kinematic analysis. Using topographic cross-sections and engineering geological model along the hazardous locations, 2D Finite Element Analysis (FEA) was carried. The rock mass parameters were updated in accordance with the findings of a back-analysis study that evaluated previous rockslope failures and analysis results jointly. The new parameters were used to conduct FEA studies of the slope's hazardous zones. Lastly, a 3D digital terrain model and RocFall3 software were used to create 3D rockfall simulations utilizng rigid body technique. Key rockfall parameters, such as the normal restitution coefficient (Rn) and the dynamic friction (ϕ), were obtained through back-analysis. 3D rockfall simulations provided falling trajectories of the failed blocks, changes in kinetic energy along these trajectories, and the bounce heights.  Based on the data obtained by the above mentioned analysis rockfall potential and risk of the region were identified. Remediation and mitigation techniques were proposed based on these findings.

How to cite: Doğu, M. M., Nasery, M. M., Ündül, Ö., and Zengin, E.: Assessment of the Risky and Hazardous Conditions of Rockfalls in Clayey Limestone with Discontinuity Control Using Integrated Analysis Methods: The Birecik – Halfet Motorway (Şanlıurfa, Türkiye), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17398, https://doi.org/10.5194/egusphere-egu26-17398, 2026.

EGU26-18844 | ECS | Orals | NH3.5

Back calculation of the 2005 Le Dar debris flow with EDDA 2.0 model: Initiation, entrainment, and deposition of a pro-/periglacial debris flow 

Marcela Vollmer-Quintullanca, Mauro Fischer, Edgar Dolores-Tesillos, and Andreas Zischg

Debris flows represent one of the major natural hazards in mountainous regions, and due to climate change, the hazard is expected to increase. With the retreat of glaciers and thawing of permafrost, new areas covered with loose material are left behind. Considering that several of these new areas have few or no recorded past events and that widely used methodological approaches are based on data from past events, the debris flow hazard assessment for these areas remains a significant challenge. Therefore, to reduce the risk related to debris flow, new methodologies and physically based models that couple the precipitation event to the initiation processes and, consequently, with the entrainment, deposition, and posterior flood, are required. 

A promising open-source, free, physically based, and depth-averaged model that targets this gap is the EDDA 2.0. This model couples precipitation intensity with infiltration and surface runoff, models slope instability and erosion by surface runoff as debris flow initiation processes, as well as the entrainment along the transition zone, deposition, and solid concentration evolution. This study evaluates the applicability of the EDDA 2.0 model for a rainfall-triggered debris flow in the Dar catchment, Switzerland. First, a comprehensive local sensitivity analysis is conducted through a one-at-a-time approach to identify the model parameters (soil and debris flow simulation) that control depositional extent, maximum flow depth at two cross-sections, and the eroded sediment volume. The sensitivity of each parameter is qualified and quantified by the screening (K1) and variance (K3) indices, respectively. From the sensitivity analysis, the model is calibrated for the 24th June 2005 event using the selected most relevant parameters. 

Our results show that the dominant parameters of the EDDA 2.0 model are the erodibility and the Manning coefficients, while the average grain size, deposition coefficient, and soil permeability play a secondary role in the analyzed outputs. The calibration process shows a good fit with the data observed after the event of the 24th of June 2005; for most of the analyzed metrics, the EDDA 2.0 model performs better than the RAMMS::DF, a widely used debris flow model in hazard assessment. While precipitation scenarios for hazard assessment are not yet included, they are part of a currently ongoing project. Preliminary modeling-with some limitations-provides us with the first insight into the challenges that must be addressed in the integration of precipitation with infiltration and erosion due to surface runoff. 

How to cite: Vollmer-Quintullanca, M., Fischer, M., Dolores-Tesillos, E., and Zischg, A.: Back calculation of the 2005 Le Dar debris flow with EDDA 2.0 model: Initiation, entrainment, and deposition of a pro-/periglacial debris flow, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18844, https://doi.org/10.5194/egusphere-egu26-18844, 2026.

EGU26-19133 | ECS | Orals | NH3.5

Near Real-time Detection of Mass Movements at an Alpine Scale 

Giulio Saibene, Dominik Amschwand, and Jan Beutel and the Rockfall Group Collaboration

The high mountain areas of the Alps are particularly sensitive to rising temperatures as expressed by the well-documented glacier loss. The link between a warming climate and the frequency of large alpine mass movements is, however, less conclusive across the Alps as a whole. Landslide and rockfall inventories are typically limited to a single class of events, localized to a specific region or research objective, available only with large delays or out of date and frequently the data contains considerable observer bias [2]. Automated and near real-time detection of large mass movements using seismic infrastructure networks have been proposed at a national level, e.g. a for Switzerland [1]. Here, a validation mechanism using an expert group of local observers is used to validate detected events post fact. This allows to (i) detect, localize and classify large rockfalls and landslides at a regional level, (ii) reduce observer bias in manually curated catalogs, and (iii) provide first quantitative analysis of events within minutes. For example, for the main collapse of the Birchgletscher/Nesthorn in Blatten CH on May 28th, 2025, the first analysis of Magnitude 3.1 was available at 15:39:37 CEST, merely 14 minutes after the event occurred. 

In this work, we first analyze the events collected and cataloged using seismic detection over the past two decades in Switzerland and bordering regions under the auspices of the Swiss Seismological Service and the Rockfall Mailing List Collaboration. In a second step, we extend this to the whole Alpine Arc with events from national seismic inventories from Switzerland, Italy, Austria, France and Germany, spanning from 1990 to present. We compare this data to catalogs derived from personal observer networks [2], scientific literature, and personal communications. Initial analysis shows that alongside the increasing temperatures and melting glaciers, the number of large mass movements in the Alps has also been rapidly increasing. A clear elevation envelope from 1000 to 4000 m is found to contain almost all of the rockfalls in the Alps and the majority of which occur in areas under permafrost conditions. The joint multi-source inventory is a first step towards a comprehensive and up-to-date statistical analysis of the impacts of climate change on the occurrence of high alpine mass movements in the Alps. 

[1] Kastli, P., Clinton, J., Kraft, T., Diehl, T., and Haslinger, F.: A near-real-time public mass movement catalogue for Switzerland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19568, https://doi.org/10.5194/egusphere-egu25-19568, 2025.

[2] PERMOS Rockfall Catalog. https://www.permos.ch/data-portal/rock-falls, accessed January 2025.

How to cite: Saibene, G., Amschwand, D., and Beutel, J. and the Rockfall Group Collaboration: Near Real-time Detection of Mass Movements at an Alpine Scale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19133, https://doi.org/10.5194/egusphere-egu26-19133, 2026.

Rockfall runout and energy dissipation are controlled by complex interactions between block characteristics and terrain properties, yet simplified approaches remain widely used for rockfall hazard assessments in the praxis. This contribution revisits the rockfall energy line method (also known as the Pauschalgefälle method), presenting its conceptual basis and an online implementation tool for estimation of rockfall velocities and kinetic energies along slope profiles. The method projects an idealised energy line from the rockfall release area to the distal margin of the deposit zone, comparable to the shadow angle approach, with modified slope angles used to approximate terrain resistance due to surface roughness and vegetation.

Despite its simplicity, the rockfall energy line method is commonly employed as a first-order estimate and plausibility check in rockfall hazard assessments. Here, we evaluate the method against data from controlled, real-world rockfall experiments and examine its performance relative to advanced numerical rockfall models. The comparison illustrates how this simplified energy-based approach can complement process-based simulations, particularly where field data are limited.

Our benchmarking highlights some limitations of the current rockfall energy line method, particularly for large, idealised blocks travelling over smooth alpine meadow terrain. Based on these findings, we propose practical adaptations to the method that improve its applicability to extreme rockfall scenarios and provide guidance for its appropriate use in rockfall hazard assessment for the praxis.

How to cite: Glover, J. and Volkwein, A.: Benchmarking and adapting the rockfall energy line method for rockfall hazard assessment , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19539, https://doi.org/10.5194/egusphere-egu26-19539, 2026.

EGU26-19753 | ECS | Orals | NH3.5

Rockfall hazard threatening archaeological sites in seismically active volcanic areas: the example of Baia Castle (Campi Flegrei) 

Luigi Massaro, Augusto Maresca, Lucia Mele, Alessandro Flora, and Antonio Santo

The Baia Castle cliff, situated in the western sector of the Gulf of Naples (within the Campi Flegrei caldera, southern Italy), is subject to ongoing geomorphological processes and cliff retreat, which threaten both the archaeological heritage and coastal infrastructure. Additionally, the periodic uplift and subsidence activity, known as bradyseism, of the caldera is often accompanied by seismic events, which, as a secondary effect, can trigger rockfalls.

This study presents a comprehensive assessment of rock mass instability at the Baia Castle cliff through high-resolution UAV-based photogrammetry, semi-automatic point cloud analysis, and traditional field surveys. The combination of remote and in-situ methods, integrated with laboratory geomechanical analysis, enabled performing a detailed geostructural characterisation and kinematic analysis of the potential failure mechanisms affecting the tuffaceous cliff. Additionally, successive drone-derived DEMs before and after the June 2025 rockfalls that occurred in the area were compared to quantify the mobilised volumes and the cliff retreat. Furthermore, the failure events of 2025 were compared with the geostructural results preceding the rockfall and with the seismic site response analysis, to investigate any potential predisposing factors that localised the rockfall detachment.

How to cite: Massaro, L., Maresca, A., Mele, L., Flora, A., and Santo, A.: Rockfall hazard threatening archaeological sites in seismically active volcanic areas: the example of Baia Castle (Campi Flegrei), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19753, https://doi.org/10.5194/egusphere-egu26-19753, 2026.

Glaciers in the Karakoram range are known to surge periodically, often triggering glacial lake outburst floods (GLOFs). However, the Shyok Valley remains comparatively understudied in this context. This study examines the surge dynamics of five glaciers- Aktash, Kichik Kumden, Chong Kumden, South Rimo-X, and Central Rimo, in the upper Shyok Valley of the Eastern Karakoram range, mapping their movements and the formation of associated lakes caused by ice-dammed river blockages. Between 1996 and 2025, three distinct lake sites formed. Two of these lakes filled and drained multiple times, while the third filled and drained only once. In total, six major outburst events and several minor drainage events were identified, including multiple previously undocumented events. While glacier surging is generally understood to follow cyclical behaviour, no consistent recurrence interval was observed in this study. Notably, GLOF locations were found to repeat, driven by the same glaciers periodically surging and obstructing the same river channels. The estimated lake volumes are comparable to those of known GLOF-producing lakes in the western Karakoram. These glaciers pose notable flood hazards due to their potential for large-scale ice dam formation and subsequent outbursts. Overall, this study contributes to further understanding of glacier surge dynamics in the eastern Karakoram, the GLOF hazards they pose and the likelihood of these events repeating.

How to cite: Rifky, A.: From Surge to Flood: GLOF Hazards Linked to Glacier Surges in the Upper Shyok Valley , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1172, https://doi.org/10.5194/egusphere-egu26-1172, 2026.

EGU26-2857 | ECS | Posters on site | CR5.7

Investigating Relationships between Lake Drainages and Surge Motion through Modeling in the Karakoram Himalaya 

Neosha Narayanan, Winnie Chu, Aleah Sommers, Colin Meyer, Jakob Steiner, and Brent Minchew

Glacier motion, retreat, and hazards like surges and glacial lake outburst floods (GLOF) are strongly affected by subglacial hydrology. In High Mountain Asia, surges and GLOF, which have caused billions in damages in recent decades, occur in the context of increasingly negative mass loss, erratic weather patterns, and dwindling water resources. While surges and GLOF have generally been studied separately, observations at surge-type glaciers in the Karakoram Range of Pakistan exhibit identical patterns of concurrent surge termination and GLOF, implying that both phenomena may be connected to changes in subglacial hydrology. Here, we build on previous modeling work with SHAKTI (Subglacial Hydrology and Kinetic, Transient Interactions) that demonstrated that seasonal subglacial hydrology alone is insufficient to explain observed velocity changes. We use a coupled subglacial hydrology and ice dynamics framework to investigate how ice-dammed lake outbursts affect the motion of surging glaciers. We then demonstrate the effects of lake bathymetry and glacier geometry on flood characteristics and ice motion.

How to cite: Narayanan, N., Chu, W., Sommers, A., Meyer, C., Steiner, J., and Minchew, B.: Investigating Relationships between Lake Drainages and Surge Motion through Modeling in the Karakoram Himalaya, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2857, https://doi.org/10.5194/egusphere-egu26-2857, 2026.

EGU26-5448 | ECS | Orals | CR5.7

Linking GLOFs at ice-dammed lakes in Greenland to ice configuration: The case of Lake Tininnilik 

Jonas Köhler and Kristian Kjeldsen

Glacier lake outburst floods (GLOFs) from ice-dammed lakes in Greenland are significant hydrological events that have a far-reaching impact on downstream ecosystems, infrastructure and glacier dynamics. A notable example is Lake Tininnilik in western Greenland, which is dammed by the marine-terminating Saqqarleq Sermia. The lake has a history of rapid drainage events involving water volumes of ~1.5 km³ and sudden drops in water level of ~65 m. Glacier thinning has increased the lake's drainage frequency from ten to five years, as evidenced by the 2010 and following GLOFs. The most recent event was observed in late July 2025.

However, GLOFs at Lake Tininnilik vary considerably in timing from year to year, depending on the configuration of the ice, while the trigger factors appear to change between ice-dam flotation and increased glacier velocity. This raises questions regarding the interplay between glacier dynamics and lake drainage processes.

Here, we present a comprehensive analysis of the relationship between the recent and historical drainage behaviour of Lake Tininnilik (occurrence, frequency and volume) and the configuration of the ice (particularly velocity and thickness) by combining time series of remotely sensed lake and ice parameters.

As part of the LIDL (Linking Ice-Dammed Lake Drainage to Ice Dynamics in Greenland) project, our aim is to apply the developed analysis framework to a wide range of ice-dammed lakes in Greenland exhibiting GLOF behaviour. Our goal is to gain a broader understanding of the role of ice flow dynamics, particularly ice thickness and velocity, in modulating and potentially initiating drainage events. This will contribute to improved GLOF prediction in a changing climate.

How to cite: Köhler, J. and Kjeldsen, K.: Linking GLOFs at ice-dammed lakes in Greenland to ice configuration: The case of Lake Tininnilik, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5448, https://doi.org/10.5194/egusphere-egu26-5448, 2026.

EGU26-6733 | ECS | Orals | CR5.7

Evidence of extreme debris flows during early Holocene glacier retreat in the Cordillera Blanca (Peru) : paleo-GLOF hypothesis and implications for current hazard 

Ronald Concha, Swann Zerathe, Benjamin Lehmann, Julien Carcaillet, Fabrizio Delgado, Dulio Gómez, Juan C. Tórres Lázaro, Diego Cusicanqui, Luis Albinez, and Manuel Cosi

The Peruvian Andes are among the world’s regions most affected by global warming, leading to rapid glacier retreat. The Cordillera Blanca (CB), the most glaciated tropical range, has lost ~41% of its glacier area since 1962. This retreat has preconditioned the formation and growth of numerous glacial lakes, increasing Glacial Lake Outburst Floods hazard and associated slope instability. The Santa River valley (western flank of the CB) is the second most exposed region worldwide to GLOFs, where steep topographic gradients favor high-magnitude floods toward downstream communities. Over the last decades, repeated catastrophic GLOFs in the Santa River valley have caused thousands of fatalities, including the 1941 Palcacocha GLOF (~1800 fatalities).

This study focuses on the Llullán and Parón valleys in the northern CB. These catchments include Laguna Parón (~60 × 10⁶ m³), considered one of the potentially dangerous glacial lakes, as well as Huandoy peak (6343 m a.s.l.). At the outlet of the Llullán valley lies an extensive fan-shaped deposit, ~4 km wide and 3 km long. The city of Caraz (~2300 m a.s.l.), with ~22,000 inhabitants, is built on this landform, where numerous very large boulders (up to 20 m in diameter) are scattered all across the surface. These features raise key questions about the magnitude and return periods of the extreme events. Our objective is to constrain the timing, magnitude, and topoclimatic conditions of the paleo-events that formed the Caraz fan deposit to assess exposure under current conditions.

Field and remote sensing observations show that the Caraz fan deposit is continuously connected to a sedimentary fill in the Llullán Valley. This surface exhibits a homogeneous longitudinal profile of ~11 km with ~5° slope, following an east–west trajectory. We inventoried hundreds of granodiorite boulders embedded across the deposit surface, which spatial and statistical distribution provide evidence of a high-energy event. Outcrops along the Santa River reveal vertical sections of a homogeneous debris-flow body characterized by subrounded granodiorite clasts (up to 5 m), some displaying jigsaw-clast structures, within a sand–gravel–silt matrix. Debris-flow run-up along the Llullán valley reached >50 m above the current riverbed, further indicating a high-energy event. The deposit ranges from 20 to 40 m in thickness, covers ~12 km², and has an estimated volume >400 × 10⁶ m³.

Twenty-four paired ages based on in-situ cosmogenic nuclide exposure dating (¹⁰Be, ²⁶Al) on eleven large boulders (including two replicates) reveal a consistent exposure history, indicating the Caraz paleo-event occurred as a single event at ~10 ka. This timing coincides with Early Holocene warming and rapid glacier retreat (horizontal velocity 4–8 km/ka) following the Younger Dryas glacial advance. We hypothesize that a paleo-lake, trapped behind the Younger Dryas moraine in the upper Parón Valley, at a location like the current Laguna Paron, may have been the source of an extreme GLOF that generated the Caraz debris-flow. Understanding the origin of the Caraz paleo-debris-flow provides key analogues to assess the hazard posed by Laguna Parón and its moraine dam, which has a volume of comparable magnitude.

How to cite: Concha, R., Zerathe, S., Lehmann, B., Carcaillet, J., Delgado, F., Gómez, D., Tórres Lázaro, J. C., Cusicanqui, D., Albinez, L., and Cosi, M.: Evidence of extreme debris flows during early Holocene glacier retreat in the Cordillera Blanca (Peru) : paleo-GLOF hypothesis and implications for current hazard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6733, https://doi.org/10.5194/egusphere-egu26-6733, 2026.

EGU26-7114 | Orals | CR5.7

Frontiers in GLOF research and risk management 

Christian Huggel, Simon Allen, Holger Frey, Evan Miles, and Laura Niggli

The last ca. 10 years have seen a particularly strong proliferation of research around glacier lake outburst floods (GLOF), with the number of corresponding peer-reviewed publications hitting 100 per year most recently.

Major progress has been made, and debates have developed, around the number, volume and change of glacial lakes, and the frequency of GLOF’s over time and the relation to glacier shrinkage and climate change, globally and in particular regions such as High Mountain Asia. Hazard and risk assessments have been performed widely, ranging from local to global scale, and against a range of climatic and socio-economic future scenarios. Major GLOF events and disasters such as the 2023 South Lhonak GLOF, have been carefully analyzed with an objective to better understand physical processes and impacts. GLOF’s are increasingly sketched as cascading processes, and thus posing important challenges to process understanding, modeling and forecast. A range of models have been applied to GLOF processes, from physically based models for local scale to simpler models at regional scale but important challenges remain.

Against this impressive progress in GLOF research, we identify and discuss here critical fields that have not yet received sufficient attention but have important scientific or societal relevance, or represent research areas where progress is facing important challenges and barriers. Specifically, we identify four core frontiers in GLOF research and risk management:

(1) Location and dynamics of hazard sources: recent cases have shown that GLOF’s often originate from poorly or unknown, or rapidly changing sources, thus posing a major issue for comprehensive hazard and risk analysis.

(2) Probability of occurrence of GLOF’s and GLOF-triggering mass movements such as rock / ice avalanches. Limited research has addressed this issue, and if, typically remained at a qualitative level. Quantification, however, will prove to be essential for areas such as climate litigation cases, for advancing probabilistic hazard and risk assessments, and as a basis for establishing risk transfer mechanisms like insurances.

(3) Several events have shown the eminent importance of sediment entrainment and flow dynamics for the impact of GLOF’s on population and infrastructure, but many challenges remain in terms of process understanding, modelling and assessment methods.

(4) Effectiveness of risk management and climate change adaptation for GLOFs: quite a range of disaster risk reduction measures for GLOF’s are recognized and global experiences have been recently comprehensively analyzed. However, as we further move into a rapidly changing high-mountain landscape, and public finance is increasingly stressed, the assessment of effectiveness and limits of risk management option against different levels of warming and related GLOF scenarios becomes more and more urgent.

We will elaborate how GLOF research can address these frontiers and what it may entail in terms of international cooperation. 

How to cite: Huggel, C., Allen, S., Frey, H., Miles, E., and Niggli, L.: Frontiers in GLOF research and risk management, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7114, https://doi.org/10.5194/egusphere-egu26-7114, 2026.

EGU26-8068 | ECS | Posters on site | CR5.7

Toward modelling glacier lake outburst floods from ice-dammed lakes: case study in Rembesdalskåka, Norway 

Léa Rodari, Pascal Emmanuel Egli, Samuel Cook, Thomas Zwinger, and Ann Victoria Rowan

Outbursts from ice-dammed lakes typically recur through cycles of filling and are driven by complex drainage mechanisms that can influence the magnitude and the timings of the Glacial Lake Outburst Flood (GLOF). Predicting GLOFs from ice-dammed lakes is complex, because ice dams are formed by an active glacier that is constantly changing in response to climate. New approaches combining numerical modelling, AI-driven models and remote sensing can be used to understand these protean hazards. This study combines subglacial modelling (using GlaDS within Elmer/Ice) with novel field data to enhance the understanding of physical processes during outburst flood events from an ice-dammed lake in Norway. This aim fits within the larger CryoSCOPE project that seeks to integrate machine-learning with physics-based numerical models and remote-sensing observations to improve the assessment of cryospheric hazards. The study glacier is Rembesdalskåka, the largest outlet glacier of Hardangerjøkulen ice cap in southern Norway and the source of Norway's most destructive GLOFs in 1893 and 1937. The glacier was monitored over the last 50 years, making an ideal case study to improve understanding of these complex processes at place. We will present field observations from 2025, and the data inputs for the modelling of GLOFs between 2023 and 2026 as a first step towards understanding the exact sequence of events and interplay of processes that drives GLOF-events at Rembesdalskåka.

How to cite: Rodari, L., Egli, P. E., Cook, S., Zwinger, T., and Rowan, A. V.: Toward modelling glacier lake outburst floods from ice-dammed lakes: case study in Rembesdalskåka, Norway, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8068, https://doi.org/10.5194/egusphere-egu26-8068, 2026.

EGU26-10127 | Orals | CR5.7

Seismic and piezometric signature of the natural drainage of the Tête Rousse glacier, august 9th 2025 

Eric Larose, jakub Kokowski, Olivier Gagliardini, Emmanuel Thibert, Julien Brondex, Stéphane Garambois, Mylène Bonnefoy, Alexis Buffet, Laurent Arnaud, Olivier Laarman, and Baptiste Camus

The Tête Rousse glacier, located in the Mont Blanc massif (French Alps), is a polythermal glacier that hosts a water pocket in the center that has been identified and monitored since around 2008 [1,2]. Despite repeated artificial pumping operations aimed at draining this cavity, it continues to retain water  and is therefore subject to regular monitoring, notably through piezometric pressure measurements, Nuclear Magnetic Resonance (NMR) surveys and ground-penetrating radar profiles. This water storage may develop into catastrophic glacial lake outburst floods (GLOF), threatening infrastructures and human lives downstream.

A seismic ambient noise campaign conducted in 2022 [3] revealed anomalies the upper part of the glacier, suggesting the presence of a second water reservoir with undefined contours. The NMR survey of 2023 confirmed the presence of around 50,000 m3 of liquid water beneath the upstream part of the glacier. However, additional GPR profiles and drillings have have left significant uncertainties about this new reservoir.

In August 2025, numerous concentric cracks were observed in the upstream sector of the glacier. On 10 August 2025, eyewitnesses reported abnormal activity in the glacier's outlet stream for several hours. The presence of piezometric sensors within the glacier, combined with recordings from a seismic sensor located at its centre, made it possible to accurately reconstruct the chronology of the drainage. Beginning on 9 August, a progressive increase in anomalous microseismic activity was observed, culminating in a main event of seismic magnitude 0. Subsequently, piezometric levels exhibited a two-stage evolution: first, water flowed from the upstream part to the central cavity; second, drainage proceeded from the central cavity toward the downstream part of the glacier. These hydrological transfers were confirmed by a second seismic proxy, namely variations in seismic background noise levels. Following the drainage event, abnormal elevated microseismic activity was observed for several weeks, reflecting the collapse of drained areas and the ongoing brittle deformation within the glacier, including the development of surface cracks.

These observations suggest that seismological monitoring and piezometric measurements constitute complementary and effective tools for understanding the dynamics of glacial water pocket drainage. Moreover, they provide several precursor and early-warning signals that could be used for monitoring strategies and operational alert systems aimed at mitigating this type of glacial hazard.

References:

[1] Vincent, C., Descloitres, M., Garambois, S., Legchenko, A., Guyard, H., & Gilbert, A. (2012). Detection of a subglacial lake in glacier de Tête

Rousse (Mont Blanc area, France). Journal of Glaciology, 58(211), 866–878.

[2] Vincent, C., Garambois, S., Thibert, E., Lefèbvre, E., Meur, E. L., & Six, D. (2010). Origin of the outburst flood from glacier de Tête Rousse in

1892 (Mont Blanc area, France). Journal of Glaciology, 56(198), 688–698.

[3] A. Guillemot, N. Bontemps, E. Larose, D. Teodor, S. Faller, L. Baillet, S. Garambois, E. Thibert, O. Gagliardini, C. Vincent : Investigating Subglacial Water-filled Cavities by Spectral Analysis of Ambient Seismic Noise : Results on the Polythermal Tête-Rousse Glacier (Mont Blanc, France), Geophys. Res. Lett. 51 e2023GL105038 (2024).

How to cite: Larose, E., Kokowski, J., Gagliardini, O., Thibert, E., Brondex, J., Garambois, S., Bonnefoy, M., Buffet, A., Arnaud, L., Laarman, O., and Camus, B.: Seismic and piezometric signature of the natural drainage of the Tête Rousse glacier, august 9th 2025, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10127, https://doi.org/10.5194/egusphere-egu26-10127, 2026.

EGU26-10959 | Orals | CR5.7

The geomorphological impact of the 1967 Steinsholtshlaup Glacial Lake Outburst Flood 

Þorsteinn Sæmundsson, Greta Wells, and Daniel Ben-Yehoshua

The overall aim of this paper is to assess the present day geomorphological record of the 1967 Steinsholtshlaup in Iceland to understand better the event and the hazards it generated, its long-term legacy and the implications for both landscape interpretation and hazard planning in areas of contemporary valley glaciation. The 1967 landslide was a complex paraglacial response to decades of down wasting of the Steinsholtsjökull glacier. The rockslide incorporated glacier ice, then swept into a proglacial lake and a confined pro-glacial valley, leaving a trail of ice, rock debris and landscape transformation. About 5 km from the site of the collapse, boulders up to 80 m3 in size were scattered immediately beyond the confluence of the proglacial valley with a wide sandur. A paper published by Kjartansson in 1967 recorded the immediate aftermath of the GLOF, but left many questions unanswered, and there have been no subsequent publications.

A better understanding of this event is important because, circumstances similar to those found in the Steinsholtsdalur valley prior to 1967 have developed in numerous glacial environments around Iceland’s ice caps.  As in many other mountain areas, increased temperatures over the last deccadees have driven renewed and rapid retreat of valley glaciers. Across Iceland, existing proglacial lakes have expanded, and many new ones have formed. These glacier fluctuations have affected the stability of neighbouring mountain slopes, which are resulting in slope deformation and mass movements. The potential for a major geomorphological incident in areas that both attract tourists year-round and have seen a recent related infrastructure development raise serious concerns and stresses an urgent need to study and monitor these environments.

How to cite: Sæmundsson, Þ., Wells, G., and Ben-Yehoshua, D.: The geomorphological impact of the 1967 Steinsholtshlaup Glacial Lake Outburst Flood, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10959, https://doi.org/10.5194/egusphere-egu26-10959, 2026.

EGU26-11346 | ECS | Posters on site | CR5.7

Remote Sensing Reconstruction and Mechanism Analysis of the July 2025 Glacial Lake Outburst Flood (GLOF) at the Gyirong Port, China-Nepal Border  

Xingdong Li, Haitao Zhang, Jie Mu, Wenlong Song, Yongmin Yang, and Fuxin Chai

Glacial retreat in the Himalayas has led to more frequent glacial lake outburst floods (GLOFs), which often pose serious transboundary threats. On July 8, 2025, a GLOF occurred in the Donglin Zangbo Basin near Gyirong Port, triggering a large-scale debris flow across the China-Nepal border. Due to the lack of field data in this remote area, we reconstructed the disaster process using multi-source remote sensing and high-resolution Gaofen-7 (GF-7) terrain data. Our analysis shows the lake expanded rapidly to 0.6  km2. By establishing a water level–area–capacity (L-A-V) relationship, the total storage was estimated at 8.0-8.5 × 106 m3, with a released volume of 5.0-6.0 × 106 m3. Based on remote sensing-derived breach morphology, the peak discharge was calculated at 1100-1400 m3, showing high consistency with downstream hydrological records. Notably, a distinct discrepancy between the estimated outburst volume and downstream flood hydrographs suggests complex subglacial hydrological mechanisms, specifically the "bulking effect" caused by intense sediment entrainment and potential englacial drainage. These findings underscore the non-linear amplification of GLOF disaster chains and demonstrate the indispensable value of remote sensing in hazard assessment.

How to cite: Li, X., Zhang, H., Mu, J., Song, W., Yang, Y., and Chai, F.: Remote Sensing Reconstruction and Mechanism Analysis of the July 2025 Glacial Lake Outburst Flood (GLOF) at the Gyirong Port, China-Nepal Border , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11346, https://doi.org/10.5194/egusphere-egu26-11346, 2026.

There is a clear link between global warming and the increase in glacier melting, leading to the expansion of glacial lakes, often dammed by fragile moraines. Triggers such as heavy rainfall, earthquakes, landslides, avalanches, glacier breakoffs, or thawing permafrost can cause glacial lake outburst floods (GLOFs). These events result in moraine breaches, releasing flood waves of mud and debris that can cause significant damage and endanger populations. On August 16, 2024, a GLOF from the Thyanbo glacial lakes affected the village Thame, Nepal. This flood caused destruction of the local infrastructure, buildings and agricultural land, and displaced over 135 inhabitants. According to first investigations, it seems that an initial trigger originated from the upper glacial lake and overtopped its terminal moraine. This flood wave further ran into the lower glacial lake, which overtopped the terminal moraine and caused it to breach. All mentioned cascading incidents triggered the GLOF running downstream. As no in situ data is available, we used high-resolution optical as well as Synthetic Aperture Radar (SAR) remote sensing data to map the lakes dynamics and measured the ground deformations at the terminal moraines. To date, such analyses have been applied only to glacial lakes and terminal moraines without documented GLOF events, but not to systems affected by a previously occurred GLOF.

High-resolution PlanetScope multispectral images from 2019 to 2024 showed an expansion of the upper lake by 213.3 % before the event, followed by a loss of 25.9 %, while the lower lake just increased slightly by 2.8 % over the timeseries, but lost over 74.3 % of its area during the GLOF. The analysis showed that the upper terminal moraine has not eroded at all or only very slightly, whereas the lower moraine has largely eroded. Consequently, while the lower lake no longer represents a future hazard, the upper lake continues to pose a high risk.

SAR Sentinel-1 images from 2020 to 2024 were used to perform a Persistent Scatterer Interferometry (PSI) with the Stanford Method of Persistent Scatterers (StaMPS). By combining ascending and descending orbits, the vertical and horizontal movements of the resulting scatterers were deconstructed. As the GLOF was likely triggered by an external factor, no abrupt movements were detected in advance by the PSI. Nevertheless, significantly stronger vertical and horizontal subsidence was observed at the lower terminal moraine, reflecting its greater exposure to the GLOF relative to the upper moraine. The analysis demonstrated that, with certain improvements, remote-sensing data combined with PSI can be used to assess the overall stability of terminal moraines and enable meaningful comparisons between them.

Based on this case study, the methodology will be transferred to a regional approach in the Himalayas in a future study to contribute to a more comprehensive inventory of potentially dangerous glacial lakes by adding the parameter of terminal moraine stability, which has not yet been considered in depth.

How to cite: Dedring, N., Rienow, A., and Graw, V.: Persistent Scatterer Interferometry for early detection of Glacial Lake Outburst Floods: A case study of the 2024 Thyanbo GLOF near Thame, Nepal, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13179, https://doi.org/10.5194/egusphere-egu26-13179, 2026.

EGU26-13281 | ECS | Posters on site | CR5.7

Glacial lake development and outburst flood hazard at Sólheimajökull glacier, Iceland 

Greta Wells, Þorsteinn Sæmundsson, Eyjólfur Magnússon, Guðfinna Aðalgeirsdóttir, and Finnur Pálsson

Glacier retreat is projected to continue with future climate warming, expanding proglacial lakes and increasing the risk of mass movement events such as landslides or rock falls. If a mass movement enters a lake, it may generate a displacement wave or glacial lake outburst flood (GLOF), which can significantly modify landscapes and threaten communities and infrastructure downstream.

Mass movement-triggered GLOFs pose an emerging yet understudied hazard in Iceland. One such site is Sólheimajökull, an outlet glacier of the Mýrdalsjökull ice cap in south Iceland that is one of the country’s most visited spots for glacier hikes and lake tours. This study presents results from new field surveys of lake bathymetry and subglacial topography to: 1) report lake volume evolution from 2009 to 2023; 2) project future lake development scenarios under continued glacier retreat; and 3) identify areas with high topographic potential of sourcing mass movements that could trigger a GLOF.

Sólheimajökull’s proglacial lake has grown significantly since it began to form around 2007, covering ~0.45 km2 by 2023. If the glacier terminus continues to retreat, the lake will expand into an overdeepened trough, roughly doubling its maximum depth, quadrupling its surface area, and increasing its volume by a factor of nine. If recent retreat rates continue, Sólheimajökull’s terminus could enter the deepest part of the trough in approximately a decade and retreat out of the lake basin within a century, though this could occur more quickly if calving rates increase due to deeper water. The estimated maximum lake extent will reach ~4 km up-valley from its current location, extending beneath several zones of the valley walls with high topographic potential of sourcing a rock fall or avalanche that could trigger a GLOF. This has significant implications for future glacier access, tourism planning, infrastructure development, and visitor risk exposure. These results can inform hazard mitigation strategies at Sólheimajökull, as well as guide studies of this emerging hazard at other proglacial lakes in Iceland.

How to cite: Wells, G., Sæmundsson, Þ., Magnússon, E., Aðalgeirsdóttir, G., and Pálsson, F.: Glacial lake development and outburst flood hazard at Sólheimajökull glacier, Iceland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13281, https://doi.org/10.5194/egusphere-egu26-13281, 2026.

EGU26-13968 | ECS | Orals | CR5.7

Modelling Erosional Dam Breach & Downstream Flood Exposure from Cascading Multi-Glacial Lake Outburst Processes in the Eastern Himalayas 

Arindam Chowdhury, Sazeda Begam, Tomáš Kroczek, Vít Vilímek, Milap Chand Sharma, and Sunil Kumar De

Rapid retreat of glaciers due to global warming has led to the expansion of glacial lakes, heightening the risk of glacial lake outburst floods (GLOFs), which pose severe threats to lives and infrastructure in downstream regions. In the Sikkim Himalaya, the Gurudongmar Lake Complex (GLC) consists of four lakes holding approximately 148 × 10⁶ m³ of water, with an enlargement rate of 74 ± 3%. This study integrates a two-dimensional erosion-based moraine-dam breach model using TELEMAC 2D and SISYPHE with one-dimensional inundation modelling in HEC-RAS to assess the impacts of multi-lake GLOFs under varying scenarios. Simulations based on remote sensing and field data revealed that in the most extreme case – an 80% overtopping breach – peak flood discharges could reach up to 8882.0 m³/s, releasing a total water volume of 59.4 × 10⁶ m³. Flood heights under these scenarios could significantly exceed those observed during the South Lhonak GLOF event of October 2023, intensifying risks for downstream communities. The assessment of 19 settlement sites using a 15×15 m fishnet revealed that Thangu Valley and Chungthang town are most vulnerable, with potential inundation levels and infrastructure exposure highest in these areas. Combined breaches, such as the sequential failure of lakes GL-2 and GL-1 or GL-3 and GL-1, further amplify the flood risk, underscoring the complex dynamics of multi-lake outbursts. This research provides critical insights into moraine-dam erosion processes and downstream flood impacts, offering a robust framework for hazard mitigation in the Eastern Himalayas and similar glacierized terrains worldwide.

Keywords: Glacial lake outburst floods (GLOFs); Erosion dam breach model; Hydrodynamic flood modelling; HEC-RAS; Exposure assessment; Sikkim.

How to cite: Chowdhury, A., Begam, S., Kroczek, T., Vilímek, V., Sharma, M. C., and De, S. K.: Modelling Erosional Dam Breach & Downstream Flood Exposure from Cascading Multi-Glacial Lake Outburst Processes in the Eastern Himalayas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13968, https://doi.org/10.5194/egusphere-egu26-13968, 2026.

EGU26-14396 | ECS | Orals | CR5.7

Glacial lakes at the Juncal catchment, Chilean Central Andes: origin, evolution and GLOF hazard management challenges 

Felipe Ugalde, Daniela Carrion, Francisco Fernandoy, and Luis Muñoz

The Juncal catchment, located in the Valparaíso Region, Central Andes of Chile, hosts 79 glaciers, including Monos de Agua and Juncal Norte glaciers. The latter has an active glaciological monitoring at least since 2020, which has allowed an accurate assessment of its recent evolution. On a regular basis, research at this site has focused on the hydrological significance both to the Region and for the Aconcagua River. Nonetheless, glacier hazards have received less attention, posing an opportunity for new studies.

In this contribution, we present the chronological evolution of three glacial lakes that originated in the Juncal catchment: (1) Juncal Norte Glacier (DGA code CL105400072A) proglacial lake, at 2,940 m a.s.l.; (2) proglacial lake 077, located in front of the CL105400077 Glacier at 3,560 m a.s.l., and (3) glacial lake 088, associated with the rock glacier CL105400088, at 4,055 m a.s.l., which is currently drained.

Through the analysis of Sentinel-2 and PlanetScope imagery, we determined that these lakes formed at the end of the 2018 boreal summer, whilst their expansion is still ongoing. By the end of 2025 summer, the extension of Juncal Norte and 077 glacial lakes reached 4 and 2 ha, respectively, whereas the 088 lake would have reached a maximum extension of 2.1 ha by May 2023. Our results show that the 088 glacial lake drainage began at the start of the summer of 2024, ending by February 2024. Special attention is given to the 077 glacial lake’s expansion, which is confined by the glacier’s frontal moraine, and is located 800 m above the river drained from the Juncal Norte Glacier. Such a condition is critical in the scenario of a GLOF, due to the high potential energy involved in an eventual outburst.

The morphological heterogeneity of these glacial lakes, combined with their location and the particular characteristics of the glaciers that originate them, poses important challenges for field surveys and the precise evaluation of the GLOF hazard assessment within the Juncal catchment.

How to cite: Ugalde, F., Carrion, D., Fernandoy, F., and Muñoz, L.: Glacial lakes at the Juncal catchment, Chilean Central Andes: origin, evolution and GLOF hazard management challenges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14396, https://doi.org/10.5194/egusphere-egu26-14396, 2026.

EGU26-16390 | ECS | Posters on site | CR5.7

Geomorphic processes of unreported GLOF cascade and past avalanches, Jammu and Kashmir, Western Himalaya 

Ashim Sattar, Shashi Kant Rai, Adam Emmer, Sunil Dhar, and Umesh Haritashya

The Warwan sub-basin in Jammu and Kashmir is a remote glaciated basin that harbors several glacial lakes and has also been showing development in terms of infrastructure and population. This sub-basin witnessed several mass movement events in the past, including avalanches and GLOF that remained unreported. This study investigates past mass movement events in the Warwan sub-basin, Jammu and Kashmir, Western Himalaya. Three major avalanche events occurred in the last two decades. The September 2005 and September 2020 avalanches occurred from glaciers GL-B and GL-A, respectively, in the same glacier complex. The March 2020 event was a rock-ice avalanche that originated from the headwall of the glacier (GL-F) located in the valley opposite the glacier complex. The avalanche terminated before reaching the ablation zone of the glacier. Mapping of the avalanche runouts revealed that the September 2020 ice avalanche initiated from the headwall of the glacier (GL-A), impacting the lake located at its terminus, causing downstream GLOF. The runout of the September 2005 rock-ice avalanche terminated before reaching the terminus, where a glacial lake started forming in 1999. Evaluation of the geomorphic processes in the glacier complex shows sediment influx through meltwater stream of GL-D and GL-E into the lake associated with GL-A. This sediment influx led to infill of the lake basin. Further retreat of GL-A led to meltwater accumulation behind the sediment infill, creating two disconnected lakes in the same lake basin. The September 2020 avalanche impacted this lake-basin, leading to complete drainage of the infill sediment and water, causing downstream debris flow. Pre and post-GLOF imagery show that the outflow channel of the lake breached, leading to channel widening. The major GLOF outwash debris formed a prominent debris fan immediately downstream of the lake. The GLOF water discharge drained into the downstream lake (GL-B), resulting in a GLOF cascade. The study highlights how GLOF events and avalanche occurrences remain unreported due to downstream cascading processes and remote locations. The study highlights how GLOF events and avalanche occurrences may remain unreported in remote locations, possibly resulting in the underestimation of a threat for downstream areas. The history of mass movement events and the growth of the glacial lakes and GLOFs in the Warwan sub-basin call for monitoring and risk assessment considering changing conditions in future.

EGUsphere preprint: https://doi.org/10.5194/egusphere-2025-6281

How to cite: Sattar, A., Rai, S. K., Emmer, A., Dhar, S., and Haritashya, U.: Geomorphic processes of unreported GLOF cascade and past avalanches, Jammu and Kashmir, Western Himalaya, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16390, https://doi.org/10.5194/egusphere-egu26-16390, 2026.

EGU26-16489 | ECS | Posters on site | CR5.7

Low-Cost Sonar-Based Bathymetry for Morphometric Analysis of Himalayan High-Altitude Lakes 

Bhawna Pathak, Ankit Singh, Nitesh Dhiman, Kirti Kumar Mahanta, and Dr. Dericks Praise Shukla

This study demonstrates the potential of cost-effective sonar integrated with uncrewed surface vehicles (USVs) for bathymetric surveys of high-altitude mountain lakes in the northwestern Himalaya, India. Three lakes were selected as test sites, Deepak Tal (3,770 m), Suraj Tal (4,777 m) near Baralacha La in Lahaul & Spiti, Himachal Pradesh, and a smaller lake near Parashar Lake (hereafter referred to as NP Lake; 2,592 m) in Mandi, Himachal Pradesh, India. The surveys were conducted using a Deeper Pro+ sonar mounted on a USV. The sonar recorded depth measurements at individual points, which were later interpolated using Kriging to generate continuous bathymetric surfaces for each lake.

For Deepak Tal, over 25,000 depth points were collected, yielding a maximum depth of 7.44 m and an estimated lake volume of 41,929.05 m³. For Suraj Tal, more than 5,000 points were acquired, with a maximum depth of 2.56 m and a corresponding volume of 9,400.95 m³. For NP Lake, approximately 1,000 points were recorded, with a maximum depth of ~1.3 m and a volume of 2,947.53 m³. Several empirical  formulas were applied to calculate volume of the lakes and compared with the field-derived volumes, revealing extremely large deviations (up to ~129,908 times), highlighting the limitations of the empirical formulas used for volume estimation of high-altitude lakes.

Overall, this study demonstrates that the Deeper Pro+ sonar mounted on a USV provides an effective, low-cost, and low-risk approach for generating high-resolution bathymetry, accurate volume estimates, and detailed morphometric information for high-mountain lakes.

Keywords: Cost-Effective Bathymetry; High-Altitude Lakes; USV; Sonar Mapping; Lake Volume; Northwestern Himalaya

How to cite: Pathak, B., Singh, A., Dhiman, N., Mahanta, K. K., and Shukla, Dr. D. P.: Low-Cost Sonar-Based Bathymetry for Morphometric Analysis of Himalayan High-Altitude Lakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16489, https://doi.org/10.5194/egusphere-egu26-16489, 2026.

EGU26-16497 | Posters on site | CR5.7

The slope of the breached channel controls potential flood volume of moraine-dammed lake outbursts 

Adam Emmer, Ashim Sattar, and Jan Hrebrina

Glacial lake outburst floods (GLOFs) originating from breaches of moraine-dammed lakes represent serious risk in high mountain regions around the world, as recently exemplified by the 2023 South Lhonak GLOF. Informed disaster risk reduction requires reliable modelling inputs. While computational capacities and modelling tools improved greatly in past years, some of the key input parameters remain poorly addressed. Among these, the estimation of realistic potential flood volume represents a major challenge. To bridge this gap, we compiled a dataset of breached moraine-dammed outbursts and calculated mean slope of the breached channel after the GLOF, as it can be used to approximate breach depth / lake level drop and so volume. The mean slope of the breached channels in the dataset varies from 2.3° (Q0) to 19.5° (Q4), while Q1 is 3.1° and Q3 is 6.6° while the median (Q2) is 5.0° and the mean is 5.5°. We found that a little change in slope of the breached channel changes estimated potential flood volume substantially, especially in cases of rather flat wide dams, suggesting high sensitivity of predictive GLOF modelling studies to this parameter.

EGUsphere preprint: https://doi.org/10.5194/egusphere-2025-4136

How to cite: Emmer, A., Sattar, A., and Hrebrina, J.: The slope of the breached channel controls potential flood volume of moraine-dammed lake outbursts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16497, https://doi.org/10.5194/egusphere-egu26-16497, 2026.

EGU26-16809 | Posters on site | CR5.7

Early detection of emergent high-mountain lakes using Sentinel-1 

Evan Miles, Stefan Fugger, Simon Allen, Jakob Steiner, and Christian Huggel

The mountain cryosphere is rapidly changing in the 21st century. Glacier mass loss is accelerating, permafrost is thawing, and precipitation falls increasingly as rain. These are fundamental changes to the hydrological functioning of high mountain catchments, including throughput and storage. There has been focused attention on the progressive development of large glacial lakes, due to their high visibility and impacts in the case of an outburst flood. Satellite-based monitoring of such sites is a relatively straightforward task, yet effective evaluation and early warning of hazards remains challenging, as it must take into account site specific considerations, the possible chains of geomorphic processes, and implementation challenges for technical, logistical, and community ownership aspects.  In recent years, however, outburst floods have increasingly occurred originating not from known large proglacial lakes, but from glacial and periglacial lakes that have developed on subseasonal timescales of weeks to months. The development of water bodies over these short timescales is often entirely unnoticed before a flood; as a result, these events have caused significant damage and fatalities, as evidenced in at least 8 distinct events in 2025. Early detection of these emergent water bodies is essential and requires a rapid-repeat operational tool that is reliable and insensitive to meteorological conditions.

In this work we develop a framework for rapid identification of anomalous water bodies using Sentinel-1 GRD data in Google Earth Engine. Sentinel-1 is frequently used in inundation mapping efforts due to the low radar backscatter of water, its cloud penetration, and short temporal revisit (6 days for 1A and 1B combined). However, the SAR data present specific challenges: distinct ascending and descending view geometries, difficulties in geocoding due to mountain terrain and glacier thinning, an uncertain backscatter threshold for lake detection, and confounding signals of wet snow, soil moisture, or seasonal vegetation development. Rather than attempting to map lakes directly, we overcome these challenges by instead identifying domains with an anomalous signal that is also consistent with water. Specifically, we determine the anomaly of the latest backscatter data to historic backscatter phenology in each pixel, expressed as a composite z-score for the ascending and descending orbits, and mapped only in domains where radar backscatter and topographic slope are both low. 

We implement this approach in our tool THAW (Transient Hydrologic Anomalies Weekly) and demonstrate its operational utility by examining the detections that would have occurred preceding the Purepu (Tibet/Nepal) and Rawoshan (Pakistan) events in 2025. In both cases, THAW identified an anomalous signal likely to indicate surface water weeks and months prior to the lakes’ drainage. The approach is not sensitive to seasonally wet snow, as it accounts for the location’s typical seasonality, but highlights the early seasonal melt of Himalayan snowpacks in 2025. Our tests at Purepu identified the growth of another lake at Nyanang Phu (Tibet), enabling an early in-situ assessment by authorities. We find this framework to complement operational lake monitoring workflows by highlighting selected domains of rapid change for expert evaluation.

How to cite: Miles, E., Fugger, S., Allen, S., Steiner, J., and Huggel, C.: Early detection of emergent high-mountain lakes using Sentinel-1, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16809, https://doi.org/10.5194/egusphere-egu26-16809, 2026.

EGU26-18261 | ECS | Posters on site | CR5.7

Timing and volume of glacial lake outburst floods in Greenland 

Florian Vacek, Faezeh M. Nick, Anneke Vries, Walter Immerzeel, and Roderik S. W van de Wal

Around Greenland more than 3300 lakes intersect with the ice sheet margin and act as natural buffer for freshwater runoff from the Greenland Ice Sheet (GrIS). More than 300 of those lakes have been identified as having drained in the past or to drain periodically. These glacial lake outburst floods (GLOFs) strongly affect the fjord ecosystem due to the large amount of freshwater abruptly entering the saline ocean environment. By draining underneath glaciers, these events affect glacier dynamics. Specifically, they can increase glacier flow velocities due to hydrostatic pressure and reduced friction at the glacier bed, permanently change the subglacial drainage system and trigger calving events due to the formation of subglacial plumes.

While the existence of these GLOF type lakes has been reported, a Greenland wide assessment of the timing, periodicity and lake volume is lacking. Here we present such an assessment conducted by leveraging open-source data, specifically Sentinel-1 radar images and the ArcticDEM strip elevation data. In Sentinel-1 radar data, water is distinguishable from other surfaces due to its characteristically low backscatter intensity. Therefore, any change in lake extent will be reflected in a change of the backscatter signal. For the 10-year period 2016-2025 and for each GLOF type lake, we create a time-series of the mean backscatter intensity over the approximate maximum lake outline. Subsequently, we detect drainages where the backscatter signal abruptly increases and stays elevated. To quantify the volume of each lake drainage, we first outline pre and post lake extents. Then, we extract the lake level by intersecting these outlines with a DEM of the lake at an empty stage. Finally, we convert lake level change to lake drainage volume by filling the DEM to the respective elevations.

We find that many lakes follow a pattern of lake drainage in the summer followed by refilling through ice sheet runoff in the following year(s). The duration of drainage cycles varies between yearly to decadal. A longer filling period is usually also associated with a larger GLOF volume. The GLOF volumes are among the largest ever reported with a magnitude of several gigatons. Furthermore, we show that the combined GLOF volumes modulate the runoff pattern of the GrIS. The runoff is buffered by filling these lakes and eventually released at a later point in time. The changing of the seasonality of freshwater reaching the ocean potentially has widespread impacts on fjord and ocean circulation, which are not captured in regional climate and ocean models.

How to cite: Vacek, F., Nick, F. M., Vries, A., Immerzeel, W., and van de Wal, R. S. W.: Timing and volume of glacial lake outburst floods in Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18261, https://doi.org/10.5194/egusphere-egu26-18261, 2026.

EGU26-18899 | ECS | Orals | CR5.7

Two Centuries of Ice-dammed Glacier Lake Outburst Floods at Rembesdalskåka, Norway. 

Ursula Enzenhofer, Erik Schytt Mannerfelt, Liss Marie Andreassen, Hallgeir Elvehøy, and Chantel Nixon

Using an ensemble of diverse data sources, including digital elevation models, lake bathymetry, mass balance records, historic texts, and regional meteorological records, we present a detailed assessment of glacier geometry and Glacier Lake Outburst Flood (GLOF) mechanism changes. The analysis focuses on GLOFs documented over the past 200 years at Nedre Demmevatn, an ice-dammed lake formed by the outlet glacier Rembesdalskåka of Hardangerjøkulen, Norway.

Our results reveal variability in glacier extent, with pronounced thinning over the past 25 years. This accelerated thinning coincides with the near-annual recurrence of outburst floods since 2014. Hydrograph data from the past decade, characterized by rapid glacier melt, indicate a shift in outburst mechanisms from overspill, partial flotation, and channel enlargement to predominantly channel enlargement. We propose that this transition is driven by seasonal temperature fluctuations, evolving lake bathymetry, and progressive thinning of the ice dam.

In total, we document 26 GLOF events over two centuries. Historical records indicate that drainage mechanisms in the 1900s alternated between supraglacial overspill and partial ice uplift with channel enlargement. The former occurred predominantly during periods of glacier advance, while the latter was more common during phases of glacier retreat, often accompanied by a reduction in ice velocity. The study reveals a link between evolving bathymetry, drainage mechanisms and glacier responses to climate warming. This knowledge is important for communities and infrastructure near rapidly changing glaciers, supporting effective adaptive strategies.

How to cite: Enzenhofer, U., Schytt Mannerfelt, E., Andreassen, L. M., Elvehøy, H., and Nixon, C.: Two Centuries of Ice-dammed Glacier Lake Outburst Floods at Rembesdalskåka, Norway., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18899, https://doi.org/10.5194/egusphere-egu26-18899, 2026.

Subaerial lakes dammed by glacier ice have a long history of scientific and public interest, as they can drain catastrophically in outburst floods (jökulhlaups) and refill repeatedly. The hazard associated with this jökulhlaup cycle may persist for decades to centuries through a cascade of processes that includes ice-dam flotation, enlargement of a subglacial drainage tunnel, and its partial or complete resealing after the flood. Theory suggests that both the height and climate-driven decay of the ice dam fundamentally control the frequency and magnitude of jökulhlaups during this cycle: thinning and retreat of the dam may lower pre-outburst lake levels and flood volumes, while reduced lake accommodation space could allow drainage events to occur more frequently, potentially several times within a single year.

Given that glacier dams have been losing elevation at accelerating rates over recent decades, I hypothesize that the jökulhlaup cycle may intensify, leading to a faster-than-linear decrease in outburst flood magnitude accompanied by an increase in jökulhlaup frequency. Testing this hypothesis has so far been constrained by sampling biases and gaps in historical flood records. Here, I present results from manual mapping of pre-outburst lake areas for at least 71 ice-dammed lakes that drained at least ten times between 1984 and 2025 in northwestern North America, Patagonia, Iceland, Scandinavia, the European Alps, and High Mountain Asia. Using optical satellite imagery from Landsat, Sentinel-2, and Planet, I systematically reconstruct jökulhlaup time series to assess decadal trends in pre-outburst lake area and drainage frequency. I fit linear and quadratic models with potential change points to test for gradual or abrupt acceleration in the jökulhlaup cycle.

Preliminary results indicate that >75% of lakes in the sample currently exhibit declining pre-jökulhlaup areas, with 15% showing evidence for an accelerated decrease in outburst magnitude. In approximately one quarter of all cases, the models favour breakpoint behaviour, with increasing pre-jökulhlaup lake areas prior to a subsequent decline. Notably, 22% of lakes have not yet reached this peak and instead show ongoing increases in pre-outburst surface area. Most of these lakes formed during the study period and actively erode their ice dams, shifting the lake toward the dam and enlarging their own basin area. This process enables lakes to buffer even high local rates of dam thinning and helps identify locations where deglaciation may favour increasing hazard, contrary to the global trend. Furthermore, only about one third of lakes show a trend toward more frequent outbursts. For most lakes, drainage frequency remains unchanged—most commonly at one event per year—consistent with the idea that subglacial tunnel systems close slowly after drainage, inhibiting multiple outbursts within a single year. Overall, the prevalence of declining outburst magnitudes occurring at largely unchanged frequencies suggests that, at the global scale, the hazard posed by ice-dammed lakes has been declining over the past four decades.

 

How to cite: Veh, G.: Smaller but not more frequent: assessing decadal trends in jökulhlaup cycle , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19116, https://doi.org/10.5194/egusphere-egu26-19116, 2026.

EGU26-21113 | Posters on site | CR5.7

Assessing the relationship between short-term meteorological variability and the timing of GLOFs in Norway based on 83 documented events 

Felix Haas, Pascal Egli, Erik Kusch, Léa Rodari, and Liss Andreassen

While the influence of long-term climatic warming on glacier lake outburst floods (GLOF) occurrence is well-documented, the role of short-term meteorological conditions in influencing the precise timing of individual outburst events remains poorly understood. This gap is particularly evident in the Scandinavian region, where only few studies have examined how variability in temperature, precipitation, and melt conditions during days and weeks prior to an outburst flood may influence the timing of GLOF events. Therefore, this study aims to systematically investigate the relationship between the short-term variability in key meteorological variables and the timing of mostly ice-dammed GLOF events in Norway. Of the 112 documented GLOF events in Norway between 1979 and 2025, only 83 were selected for further analysis, as precise event dates were not available for all documented outburst floods. Meteorological variables for all individual GLOF events were extracted using the NORA3 dataset, a reanalysis product provided by the Norwegian Meteorological Institute. Time windows of 60, 30, 15, 7, and 3 days prior to each event were defined to assess short-term changes in meteorological conditions leading up to the outburst floods. The analysis shows no clear general relationship between precipitation and timing of GLOF events. However, in a few cases, intense precipitation immediately prior to the outburst may have acted as a triggering factor. Regarding temperature development prior to the outburst events across different time windows, the analysis revealed an inverse relationship: Significant warming trends are more prevalent over longer periods preceding an outburst, whereas shorter-term windows are dominated by non-significant or negative temperature trends. A quite similar pattern was observed regarding the change of the mean average temperatures across the different time windows. Comparing the 7 days immediately prior to an outburst with the preceding 60 days, mean temperatures were higher in 66.3 % of events. In contrast, when considering the 3 days prior compared to the preceding 30 days, only 49.4 % of events were warmer. These findings suggest that short-term warming immediately before GLOFs does not follow a consistent pattern. Regarding total water input (melt and precipitation), the analysis shows no evidence of a systematic short-term increase immediately prior to outbursts. While longer periods (e.g., 15 days) preceding events often had higher cumulative input compared to earlier intervals, the proportion of events with higher input decreased for shorter time windows. Furthermore, snow cover at the glacier margins was analyzed using satellite data, revealing that the majority (54%) of glaciers remained snow-covered both before and after the outburst events. The analysis shows that no single trigger can be identified in most cases, but that a minimum amount of meltwater input combined with short-term cooling may be a combination of conditions that frequently precedes outburst floods at ice-dammed lakes in Norway.

How to cite: Haas, F., Egli, P., Kusch, E., Rodari, L., and Andreassen, L.: Assessing the relationship between short-term meteorological variability and the timing of GLOFs in Norway based on 83 documented events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21113, https://doi.org/10.5194/egusphere-egu26-21113, 2026.

EGU26-202 | ECS | Orals | CL1.2.7

Principal component analysis of the power spectra of high-resolution ice core records 

Rhys-Jasper León, Valerie Morris, Brooke Chase, Bradley Markle, Adira Lunken, Ella Johnson, Jesus Lara Rivas, Richard Nunn, Theodore Carr, Rylan Abel, Jillian Rinaldi, Laurel Bayless, and Tyler Jones

High-resolution ice core records allow for analysis of variability on short timescales (annual, sub-annual, decadal) in addition to longer timescales (centennial, millennial), as well as how variability on different timescales changes across time.  Spectral analysis of these time series data is used to evaluate the amplitudes of signals in the records at particular frequencies. Principal component analysis (PCA) is a technique for dimensionality reduction while retaining the maximum possible variance from the original data. PCA can be used with Empirical Orthogonal Functions (EOFs) to identify the dominant spatial patterns (EOFs) with their corresponding time variations (PCs). Applying this technique to the spectra of ice core records will help to explore the spatial patterns of variability in the frequency domain by identifying the dominant modes of spectral variability (PCs) and the spatial pattern of this variability across an ice sheet (EOFs).
The power spectra will be produced for a suite of high-resolution ice core water isotope records, with methodological choices for resampling resolution being informed by results from tests with synthetic data. PCA will then be applied to the dataset of power spectra, where each spectrum is an observation and the different frequency bins are the variables. This analysis will be applied to the Holocene section of the ice cores in particular, to create a more comprehensive picture of the high frequency variability on short timescales (annual, sub-annual, decadal) and regional climate dynamics. The Holocene-only focus has the ability to resolve high-frequency signals that are often lost in older ice due to ice thinning and diffusion. Further, the relatively stable Holocene climate will allow for a more focused study of the regional mechanisms in the Arctic that operate on shorter timescales. 

How to cite: León, R.-J., Morris, V., Chase, B., Markle, B., Lunken, A., Johnson, E., Lara Rivas, J., Nunn, R., Carr, T., Abel, R., Rinaldi, J., Bayless, L., and Jones, T.: Principal component analysis of the power spectra of high-resolution ice core records, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-202, https://doi.org/10.5194/egusphere-egu26-202, 2026.

EGU26-3718 | ECS | Orals | CL1.2.7

Improving the CH4 budget using new dual-isotope CH4 records over the last glacial cycle 

Michaela Mühl, Jochen Schmitt, Barbara Seth, and Hubertus Fischer

Ice core derived records of the past atmospheric methane concentration ([CH4]) and its isotopic composition (δ13C-CH4 and δD-CH4) allow us to reconstruct its past variability and its link to changes in the climate system.  During the last glacial cycle, [CH4] showed pronounced increases from glacial to interglacial conditions, but [CH4] also closely followed large and rapid millennial-scale warming events in the Northern Hemisphere associated with Dansgaard-Oeschger (DO) events, indicating the strong sensitivity of terrestrial biogeochemistry to (hydro-) climatic changes.

To better understand the climate-greenhouse gas feedback cycle and what controlled past atmospheric methane variability it is essential to quantify the response of the CH4 budget and terrestrial biogeochemistry to such abrupt climate variations. Such a budget provides a framework to infer the strength and temporal dynamics of individual CH4 sources (e.g. wetlands, biomass burning, geologic emissions). However, for most parts of the last glacial cycle a quantitative source attribution is missing or still a matter of debate.

Synchronized ice core records from both polar regions allow us to derive the Inter-Polar Difference in [CH4] reflecting latitudinal emission difference and are used to distinguish low and high latitude CH4 emissions.  Another powerful tool to uncover source contribution to the global CH4 budget is provided by records of methane’s stable isotopic composition (δD-CH4, δ13C-CH4) as CH4 released by the various sources are associated with characteristic isotopic signatures and different sinks are connected to systematic isotope fractionations.

Here we present new δD-CH4 data from bi-polar ice cores (EDC, EDML and GRIP ice core samples) covering large parts of the last glacial cycle complementing our existing δ13C-CH4 record (Möller et al., 2013).  We use δ13-CH4 and δD-CH4 as quantitative tracers of changes in the CH4 budget and interpret atmospheric signals in a simple CH4 stable isotope-enabled one-box model of the global CH4 cycle concentrating on the prominent DO-21interval between 86 kyr and 76 kyr. We derive quantitative estimates of plausible global CH4 source mix scenarios but also review in this context uncertainties arising from poorly constrained assumptions in the past. Limited knowledge of past isotopic source signatures of biogenic CH₄ sources (wetlands) and their latitudinal distribution introduces substantial uncertainty into reconstructions of the past methane budget. Because drivers of past changes remain poorly understood, uncertainties in these assumptions propagate into estimated CH₄ emissions. For the first time, dual-isotopic CH₄ records enable an evaluation of temporal changes. Building on the new dual-isotopic constraints, we go beyond previous studies and present a new Monte Carlo approach that simulates realistic past isotopic source signatures and assesses their impact on the inferred CH₄ budget.

How to cite: Mühl, M., Schmitt, J., Seth, B., and Fischer, H.: Improving the CH4 budget using new dual-isotope CH4 records over the last glacial cycle, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3718, https://doi.org/10.5194/egusphere-egu26-3718, 2026.

EGU26-3938 | ECS | Orals | CL1.2.7

Earth’s energy imbalance across an entire glacial cycle (MIS 9–7) reconstructed from noble-gas ratios in ice cores 

Markus Grimmer, Henrique Traeger, Patrice Tinner, Daniel Baggenstos, Jochen Schmitt, and Hubertus Fischer

Earth’s energy imbalance (EEI) determines whether the planet experiences a net gain or loss of energy. The ongoing surge in atmospheric greenhouse-gas concentrations, caused by burning fossil fuels and land-use change, causes a positive EEI, which ultimately drives global warming. Today, most of this excess heat is taken up by the largest, fast-responding energy reservoir that is the surface ocean. On millennial to orbital timescales, by contrast, energy partitions between two considerably larger but slower-responding reservoirs: the global (deep, intermediate, and surface) ocean and the latent heat involved in growing and melting continental ice sheets. Ocean heat content (OHC) and global sea level, which mirrors ice sheet volume, are thus key metrics to assess the global energy balance during the Quaternary.

Past OHC can be reconstructed by analyzing noble-gas ratios in polar ice-core samples. This method makes use of the temperature-dependent and species-specific solubility of noble gases in seawater, as well as their inertness, due to which the total amount of noble gases in the ocean‐atmosphere system is conserved. Earlier studies mostly focused on the last glacial Termination and other periods of interest across the last glacial cycle. Here, we present data for an entire glacial cycle (MIS 9–7) together with data over the last four glacial terminations in millennial resolution.

By combining our OHC record with past sea-level reconstructions we obtain an EEI record spanning an entire glacial cycle. This EEI record shows the expected orbital-scale variability in response to the albedo and greenhouse gas feedback, with energy fluxes partitioning approximately equally between the ocean and ice sheet reservoirs. The EEI record also manifests strong millennial power. These millennial-scale EEI features are mirrored in the OHC record, whereas the ice sheet response is delayed and subdued, indicating that the ocean is the dominant millennial-scale energy reservoir. Millennial-scale EEI and OHC variability is closely linked with changes in AMOC strength, suggesting that ocean circulation modulates EEI and OHC across different climate states. Potential AMOC weakening under future global warming may thus add to the EEI anomaly for centuries to come.

How to cite: Grimmer, M., Traeger, H., Tinner, P., Baggenstos, D., Schmitt, J., and Fischer, H.: Earth’s energy imbalance across an entire glacial cycle (MIS 9–7) reconstructed from noble-gas ratios in ice cores, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3938, https://doi.org/10.5194/egusphere-egu26-3938, 2026.

EGU26-4630 | Orals | CL1.2.7

 EastGRIP ice core mercury record over the Holecene: From the ice accumulation record to atmospheric depositional history  

Feiyue Wang, Zhiyuan Gao, Richard Oliveira, and Dorthe Dahl-Jensen

Mercury is a contaminant of global concern, but anthropogenic impact on preindustrial mercury cycling in remote locations remained poorly constrained. Here we report a high-resolution record of the mercury concentration and accumulation flux over the Holocene, established by the analysis of the recently retrieved EastGRIP ice core from Greenland. We show that the Holocene ice core mercury record was shaped by a combination of volcanic eruptions, climate excursions, and in recent millennia anthropogenic activity. Our result suggests that human activity started to impinge on Greenlandic mercury cycling since at least 2000 years ago, much earlier than previously thought. We will also discuss the challenges encountered in establishing atmospheric mercury deposition history from the ice core record due to uncertainties associated with potential changes in post-depositional processes over the Holocene.

How to cite: Wang, F., Gao, Z., Oliveira, R., and Dahl-Jensen, D.:  EastGRIP ice core mercury record over the Holecene: From the ice accumulation record to atmospheric depositional history , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4630, https://doi.org/10.5194/egusphere-egu26-4630, 2026.

EGU26-4901 | ECS | Orals | CL1.2.7

First interpretation of 17O-excess variability over 800,000 years on the East Antarctic Plateau, based on EPICA Dome C deep ice core 

Emma Samin, Amaëlle Landais, Thomas Combacal, Antoine Grisart, Jean Jouzel, Valérie Masson-Delmotte, Bénédicte Minster, Frédéric Prié, and Barbara Stenni

Analysis of water isotopes (oxygen and hydrogen) in Antarctic ice cores has enabled reconstruction of Earth’s temperature over the last 800,000 years with the EPICA deep ice core (Dome C) and, soon, over 1.5 million years with the Beyond EPICA deep ice core (Little Dome C). In parallel, differences in fractionation between hydrogen isotopes and oxygen isotopes provided information about the water cycle in the past.

In particular, deuterium excess (dxs = δD − 8 * δ18O) has been developed to track evaporation and transport conditions from oceanic regions to the ice sheet. However, it is quite challenging to deconvolute source-related and transport-related effects. The 17O-excess (17O-excess = ln(δ17O+1) − 0.528×ln(δ18O+1)) is a less known second-order parameter, complementary to dxs, also expected to reflect the conditions encountered by the air mass.

Here we present the first long-term record of 17O-excess (from 41,520 to 800,000 years, with 2,447 data points) based on the analysis of the EPICA deep ice core to better understand the long-term variability of this proxy and its integration into high-latitudes climate variability.

In addition to variations over glacial–interglacial cycles, we observe a significant decrease of the 17O-excess over the Mid-Brunhes transition ~400,000 years ago. This 17O-excess record carrying information on the origin of the moisture precipitating in East Antarctica is compared with long-term reconstructions of sea surface temperature, Antarctic circumpolar current strength, and southern westerly winds to disentangle the effects of source changes and isotopic fractionation along transport pathways.

Measuring the 17O-excess record over such a long period, and compare it with other paleoclimatic records, offers the opportunity of better understanding the variability of this proxy, but also of deepening our understanding of the relationship between climate and water cycle changes at high latitudes. 

How to cite: Samin, E., Landais, A., Combacal, T., Grisart, A., Jouzel, J., Masson-Delmotte, V., Minster, B., Prié, F., and Stenni, B.: First interpretation of 17O-excess variability over 800,000 years on the East Antarctic Plateau, based on EPICA Dome C deep ice core, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4901, https://doi.org/10.5194/egusphere-egu26-4901, 2026.

EGU26-5512 | ECS | Orals | CL1.2.7

A perspective on ancient Antarctic (blue) ice 

Veronica Tollenaar and Etienne Legrain

The Antarctic ice sample record, collected since the 1960s, covers the past 1.2 million years continuously, and contains discontinuous “snapshots” up to 6 million years. Over 40 Antarctic ice cores have vastly advanced the understanding of past climate variations and will continue to tackle key paleoclimate question in the coming decades.

To obtain and further refine the discontinuous record older than 1.2 million years, ongoing efforts are targeting so-called blue ice areas. In these areas, complex ice flow patterns can trap extremely old ice, as demonstrated in the Allan Hills region (Transantarctic mountains). However, these complex flow patterns pose challenges in the search for and interpretation of ancient ice. To overcome these challenges and further unlock this paleoclimatic archive, blue ice research advances with: (i) systematic surface dating as a preliminary step to drilling; (ii) improving the understanding of age relationships between ice, dust, and meteorites; (iii) developing models that account for the specific physical properties of blue ice to identify and characterize the oldest trapped ice; and (iv) methods for the reconstruction of the paleoclimate signals preserved within this archive. In this perspective, we discuss past and current blue ice projects and contextualize the findings in the Antarctic paleoclimate record.

How to cite: Tollenaar, V. and Legrain, E.: A perspective on ancient Antarctic (blue) ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5512, https://doi.org/10.5194/egusphere-egu26-5512, 2026.

EGU26-5517 | ECS | Posters on site | CL1.2.7

Preserving glacier climate archives in a warming world: the Ice Memory project and the Italian contribution 

Agnese Petteni, Fabrizio De Blasi, Daniele Zannoni, Andrea Spolaor, Giulio Cozzi, Giulia Vitale, Azzurra Spagnesi, Carlo Barbante, and Jacopo Gabrieli

Anthropogenic climate change is driving a widespread retreat of glaciers, which has accelerated in recent decades. By 2100, projections indicate that between 25% and 50% of global glacier mass will be lost, depending on the emission scenario [1]. This rapid decline endangers the climatic information preserved in ice layers. The international Ice Memory project aims to safeguard this natural archive by collecting paired ice cores from mid- and high-latitude glaciers [2]. One core is analysed using present-day techniques, while the second is stored in a cave at Dome C, in Antarctica, ensuring long-term access to this climatic information for future generation of scientists.

The Italian Ice Memory team focused on mid-latitude and Arctic glaciers through six dedicated expeditions. Four expeditions target high-elevation Alpine sites above 4,000 m a.s.l.: Grand Combin (attempted in 2020 and successfully in 2025, Switzerland/Italy), Monte Rosa (2021, Italy/Switzerland), and Colle del Lys (2023, Italy/Switzerland). One expedition was carried out in the Apennines at about 2,700 m a.s.l. on the Calderone Glacier (2022, Italy), and another at Svalbard on the Holthedlafonna Glacier (2023, Norway). Drilling operations were performed using an electromechanical drilling system, and a thermal drill was tested for the first time during the 2025 Grand Combin expedition. The main unexpected challenge encountered at both high- and mid- latitude glaciers was the presence of aquifers located tens of meters below the surface. The occurrence of liquid water layers reflects the polythermal feature of these glaciers, which are increasingly suffering the rising of temperatures.

The recovered ice cores will be analysed in the coming months with the novel Continuous Flow Analysis (CFA) system designed at Ca’ Foscari University, in collaboration with the Institute of Polar Science (CNR-ISP). The analyses include measurements of insoluble dust particles, organic, inorganic and emerging compounds, biochemical markers, and stable water isotopes. In addition, 210Pb- based dating and palynological indicators will be analysed using discrete methods. Together, these results will allow the reconstruction of past climate variability and atmospheric circulation patterns.

Future Italian expeditions will focus on Asia, particularly on the Karakorum (Pakistan) and the Himalaya (Nepal).

 

[1] Zekollari, H. (2024), Cryosphere 18, https://doi.org/10.5194/tc-18-5045-2024

[2] Ice Memory Foundation, https://www.ice‑memory.org

How to cite: Petteni, A., De Blasi, F., Zannoni, D., Spolaor, A., Cozzi, G., Vitale, G., Spagnesi, A., Barbante, C., and Gabrieli, J.: Preserving glacier climate archives in a warming world: the Ice Memory project and the Italian contribution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5517, https://doi.org/10.5194/egusphere-egu26-5517, 2026.

EGU26-5553 | Posters on site | CL1.2.7

The expression of climate in the Weddell Sea region in comparison to the rest of Antarctica for events in the last glacial period 

Eric Wolff, Isobel Rowell, Thomas Bauska, Mackenzie Grieman, Helene Hoffmann, Jack Humby, Robert Mulvaney, Christoph Nehrbass-Ahles, and Rachael Rhodes

The Skytrain Ice Rise ice core adds to the handful of climate records from Antarctica that cover the whole of the last glacial period (here, we consider ~100-10 ka bp). By our count 7 records have been published covering the entire period and a further 6 cover a substantial part of it. Using the synchroneity of signals across the continent (for example in components of dust and in methane) we can tie the records together temporally. The precision of such ties is good enough to allow comparison of the timing and shape of particular events across the continent.

Many of the differences between sites will derive from local changes of elevation that certainly occur at ice rise sites. We first will discuss the glacial water isotope record from Skytrain Ice Rise (in comparison to other sites) in this context.  This will supplement the work we have already done on the Holocene and the last interglacial period using the Skytrain Ice Rise core.

However we primarily focus on a number of events such as the Antarctic Cold Reversal and some of the large Antarctic Isotopic Maxima (eg AIM 12).  We will present records from the different sectors of Antarctica. We will investigate whether any sectors of Antarctica led in such events, and determine the relative amplitude of such events around the continent. This information will offer diagnostic tests to ideas about the causes and process of millennial scale variability across the glacial period.

How to cite: Wolff, E., Rowell, I., Bauska, T., Grieman, M., Hoffmann, H., Humby, J., Mulvaney, R., Nehrbass-Ahles, C., and Rhodes, R.: The expression of climate in the Weddell Sea region in comparison to the rest of Antarctica for events in the last glacial period, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5553, https://doi.org/10.5194/egusphere-egu26-5553, 2026.

EGU26-5609 | Posters on site | CL1.2.7

Optimizing Laser Ablation–CRDS Coupling for Spatially-Resolved Millimetric Isotopic Measurements on Ice Cores 

Daniele Zannoni, Marco Roman, Pascal Bohleber, and Barbara Stenni

Ice cores are extremely valuable archives of the past atmospheric composition, extending back more than 1 million years. In such ancient ice, ice layers become extremely thinned, and the spatial resolution of analytical techniques becomes the primary factor limiting the ability to resolve past climate signals, such as the temperature-related variability inferred from the stable isotopic composition of the ice. Laser ablation (LA) is a micro-destructive technique that has recently shown strong potential for coupling to cavity ring-down spectroscopy (CRDS) to retrieve the isotopic composition of ice-core samples with minimal sample loss. In principle, LA–CRDS not only enables substantially higher spatial resolution than conventional methods but has the potential to gain new insights into signal formation processes in shallow ice by mapping the two-dimensional distribution of stable water isotopes within the ice matrix. However, LA–CRDS hyphenation remains challenging due to several factors, including wavelength-dependent suboptimal laser–ice interaction that can induce isotopic fractionation during ablation, and limitations related to the fast detection of transient signals by commercially available CRDS analyzers. To address these challenges, it is necessary to identify and constrain the factors affecting the ablation efficiency and the aerosol transport between the two systems, while remaining within the operational specifications of both instruments. In the context of the Isotope iMAGing for Ice Core Science (IMAGICS) project, we investigate how laser energy density, artificial ice generation (slow and flash freezing), and measurement configuration affect the LA–CRDS efficiency using an ArF excimer laser (Analyte Excite+, Teledyne Photon Machines) coupled to a CRDS water vapor isotope analyzer (L2130-i, Picarro). Artificial ice samples with known isotopic composition were analyzed under varying laser fluence, dosage, and firing duration. The water-vapor-calibrated CRDS analyzer collected aerosol and vapor generated in the LA cell via an Aerosol Rapid Introduction System (ARIS), operated under its default sampling configuration (~40 ml min-1, 1 Hz). Preliminary results from this study indicate that, although isotopic fractionation effects are observed in the retrieved aerosol and vapor composition, as previously reported in Malegiannaki et al (2024), the high repeatability of water vapor peaks and isotopic plateaus suggests that the LA–CRDS system introduces a systematic, non-random bias. This finding implies that a correction based on tailored calibration experiments to characterize ice–laser sensitivity is feasible. Such an approach would enable reproducible and accurate isotopic analyses of ice samples with reasonable analysis times (e.g., <10 s per mm2 of ablated ice surface).

Malegiannaki, E., Bohleber, P., Zannoni, D., Stremtan, C., Petteni, A., Stenni, B., Barbante, C., Vinther, B. M., & Gkinis, V. (2024). Towards high-resolution water isotope analysis in ice cores using laser ablation - cavity ring-down spectroscopy. Analyst , 149 (24), 5843–5855. https://doi.org/10.1039/d4an01054j

How to cite: Zannoni, D., Roman, M., Bohleber, P., and Stenni, B.: Optimizing Laser Ablation–CRDS Coupling for Spatially-Resolved Millimetric Isotopic Measurements on Ice Cores, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5609, https://doi.org/10.5194/egusphere-egu26-5609, 2026.

EGU26-5661 | Orals | CL1.2.7

Identifying optimal drilling sites in Antarctic Blue Ice Areas using a flowline model 

Etienne Legrain, Veronica Tollenaar, Frank Pattyn, Maaike Izeboud, Lisa Ardoin, François Fripiat, and Harry Zekollari

Blue ice areas have attracted growing interest over the past decade, notably following the recovery of ice older than the current record of deep ice core drilling, in the Allan Hills region of Antarctica (snapshots up to 6 million of years). In this study, we assess the suitability of flowline modelling for surface age prediction in blue ice environments. To this end, we perform 10,000 theoretical experiments covering a wide range of site conditions, using an ice-dynamical flowline model, to determine which factors most strongly favor the preservation of old ice at the surface. Our results show that a strong negative surface mass balance (i.e. high ablation) and slow surface velocities along the flowline are the primary controls on the emergence of old ice at the surface, whereas ice thickness and distance from the upstream accumulation zone play only secondary roles. Moreover, based on statistical and machine learning analyses, we illustrate that the occurrence of very old ice at the surface appears to be mostly correlated with exceptionally low surface velocities, with high ablation rates being insufficient on their own. We compare these findings with recently measured surface mass balance and surface velocities in the Sør Rondane Mountains blue ice areas (Dronning Maud Land, East Antarctica) to inform the selection of future ice core drilling site in the region.

How to cite: Legrain, E., Tollenaar, V., Pattyn, F., Izeboud, M., Ardoin, L., Fripiat, F., and Zekollari, H.: Identifying optimal drilling sites in Antarctic Blue Ice Areas using a flowline model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5661, https://doi.org/10.5194/egusphere-egu26-5661, 2026.

EGU26-6202 | Posters on site | CL1.2.7

High-resolution analyses of mineral dust at Dome Fuji, Antarctica during 35-53 kyrBP 

Kumiko Goto-Azuma, Motohiro Hirabayashi, Kaori Fukuda, Jun Ogata, Hiromi Okumura, Ikumi Oyabu, Kyotaro Kitamura, Fumio Nakazawa, Shuji Fujita, Tomotaka Saruya, and Kenji Kawamura

To investigate millennial-scale variations in mineral dust and its provenance during the last glacial period, we analyzed the Dome Fuji deep ice core using a Continuous Flow Analysis (CFA) system. We measured microparticles, eight elements (Na, Mg, Al, Si, K, Ca, Fe, and S), and stable water isotopes over the depth interval from 730 to 930 m. This interval corresponds to approximately 35–53 kyr BP, encompassing Antarctic Isotope Maxima (AIM) 8 to AIM 13 and part of AIM 14. In addition to the CFA measurements, discrete samples were continuously collected at 50 cm intervals and analyzed for particle concentrations and size distributions using a Coulter Multisizer 4e.

Concentrations and fluxes of microparticles—predominantly derived from mineral dust—as well as dust-sourced elements decreased during AIM events and increased during stadial periods, consistent with previous Antarctic ice-core studies. Centennial averages of elemental concentration ratios (Ca/Al, Fe/Al, and Si/Al) exhibit only minor variations throughout this period. This behavior contrasts with the pronounced changes observed during Termination I, suggesting relatively stable dust provenance during 35–53 kyr BP. Microparticle sizes increased during AIM events and decreased during stadials, indicating changes in transport and/or deposition rather than source shifts.

How to cite: Goto-Azuma, K., Hirabayashi, M., Fukuda, K., Ogata, J., Okumura, H., Oyabu, I., Kitamura, K., Nakazawa, F., Fujita, S., Saruya, T., and Kawamura, K.: High-resolution analyses of mineral dust at Dome Fuji, Antarctica during 35-53 kyrBP, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6202, https://doi.org/10.5194/egusphere-egu26-6202, 2026.

EGU26-6988 | Posters on site | CL1.2.7

Spatial variability of climate change signature in Antarctica revealed by ice cores 

Barbara Stenni, Agnese Petteni, Mathieu Casado, Quentin Dalaiden, Joel Savarino, Andrea Spolaor, Silvia Becagli, Adrien Ooms, Niels Dutrievoz, Cécile Agosta, Elsa Gautier, Amaelle Landais, Emma Samin, Massimo Frezzotti, Elise Fourré, Giuliano Dreossi, Roxanne Jacob, Thomas Combacal, Anaïs Orsi, and Mauro Masiol

Polar amplification leads to a larger warming in polar regions compared to the global average [1]. While an overall warming is observed in West Antarctica and Antarctic Peninsula, the temperature signal in East Antarctica remains uncertain [2]. In Antarctica, atmospheric weather stations are sparse and mainly located near the coast. While state-of-the-art atmospheric reanalysis are available from 1940, the historical climate variability at the Southern Hemisphere high latitudes are mostly based on the teleconnections with low-latitude regions, as almost no high-latitude observations are available before the satellite era (i.e., 1979). This therefore introduces a discontinuity in around 1980 associated with the incorporation of satellite observations in reanalysis.

To address these limitations, ice core records provide a valuable long-term archive of past climatic conditions through the well-established relationship between water isotopes (δ¹⁸O and δ2H) and local temperature. This relationship – commonly referred to as “paleothermometer” – is widely used for reconstructing past temperature variations.

Within the framework of the East Antarctic International Ice Sheet Traverse (EAIIST, 2019–2020), a set of shallow ice cores was recovered between Concordia Station and the South Pole. Here, we present isotope records from firn cores collected at Paleo (79°38′47″S; 126°08′15″E) that we combine to the water isotopic record obtained on the 85 m firn core at Little Dome C within the Ice CORe Dating project (ICORDA, 2019–2025, see poster by Minster, Samin et al.) providing climatic information at decadal resolution in this region of the interior of the East Antarctic Plateau. By comparing these records with atmospheric reanalyses and temperature reconstructions, we observe a strong spatial contrast between the interior and the coastal region over the past few decades. This dipole pattern is characterized by a surface warming in the interior of the continent and surface cooling along the coast of Adélie Land. To isolate the local signal of anthropogenic warming, we account for the influence of large-scale atmospheric dynamics, such as the Southern Annular Mode. Furthermore, ice core evidences, combined with climate model outputs, provide a context of the current warming over the last two centuries. This permits to assess whether climate models can correctly reproduce the spatial contrast between the interior and the coastal region in terms of surface temperature multi-decadal variability, essential for reliable future projections.

Italian partners received funding from the PNRA through “EAIIST” (PNRA16_00049-B) and “EAIIST-phase2” (PNRA19_00093) projects.

 

[1] Casado M., et al. (2023), Nat. Clim. Change 13. https://doi.org/10.1038/s41558-023-01791-5

[2] Clem KR., et al. (2020), Nat. Clim. Change 10. https://doi.org/10.1038/s41558-020-0815-z

How to cite: Stenni, B., Petteni, A., Casado, M., Dalaiden, Q., Savarino, J., Spolaor, A., Becagli, S., Ooms, A., Dutrievoz, N., Agosta, C., Gautier, E., Landais, A., Samin, E., Frezzotti, M., Fourré, E., Dreossi, G., Jacob, R., Combacal, T., Orsi, A., and Masiol, M.: Spatial variability of climate change signature in Antarctica revealed by ice cores, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6988, https://doi.org/10.5194/egusphere-egu26-6988, 2026.

EGU26-8223 | Posters on site | CL1.2.7

Investigating the preservation of rapid climate signals in the ice matrix using 2D LA-ICP-MS 

Tobias Erhardt, Marko Linda, Chantal Zeppenfeld, Ilka Weikusat, Hubertus Fischer, and Wolfgang Müller

In recent years, laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) has been further developed to obtain aerosol-derived impurity records from ice core samples at sub-mm to µm resolution (Müller et al., 2011; Bohleber et al., 2020).

For thinned ice from the lower parts of ice cores, the high spatial resolution of the method in principle promises to resolve climate variability at temporal scales that are unresolvable by other methods such as continuous flow analysis. However, spatially resolved, two-dimensional maps of the impurity distribution in the ice from LA-ICP-MS have revealed the complex interplay between the impurities and the ice’s polycrystalline structure (Della Lunga et al., 2014; Bohleber et al., 2020; Stoll et al., 2023). Some impurities such as sodium, predominantly from sea salt aerosols, show very high localisation along grain boundaries. Other elements that are typically associated with water-insoluble dust aerosols such as iron, aluminium, and calcium, however, often do not show such a strong localisation but are dispersed as particles in the ice matrix.

This localisation poses the question: At what spatial and thus temporal scale the LA-ICP-MS records are interpretable as climate records? And at which scale the post-depositional processes in the ice masks the climate signal by e.g. by dynamic or static recrystallization. This is especially relevant in the context of the evolution of the ice towards generally larger crystal sizes with increasing depth within the ice sheet accompanied by the thinning of the annual layers.

To investigate the preservation of high-frequency climate variability, we applied our newly developed 157 nm cryo-LA-ICP-MS/MS setup (Erhardt et al., 2025) to ice covering the warming transition into Greenland Interstadial 1 in the EGRIP ice core at 1375 m depth. Here, we present spatially resolved impurity maps at the ~100-µm scale spanning the rapid warming transition. Bulk concentration data from continuous flow analysis of the same ice indicates that this warming transition is exceptionally fast at EGRIP, happening within only a few years. Ice-fabric data shows grain diameters increasing from 1.5 to 1.8 mm across this transition from dustier stadial to cleaner interstadial ice (Stoll et al., 2025). This makes it a good candidate to investigate the imprint of the ice matrix onto rapid climate signals in the ice-core impurity record.

 

Bohleber, P. et al. (2020) Imaging the impurity distribution in glacier ice cores with LA-ICP-MS. Journal of Analytical Atomic Spectrometry

Della Lunga, D. et al. (2014) Location of cation impurities in NGRIP deep ice revealed by cryo-cell UV-laser-ablation ICPMS. Journal of Glaciology

Erhardt, T. et al. (2025) Rationale, design and initial performance of a dual-wavelength (157 & 193 nm) cryo-LA-ICP-MS/MS system. Journal of Analytical Atomic Spectrometry

Müller, W., Shelley, J.M.G. & Rasmussen, S.O. (2011) Direct chemical analysis of frozen ice cores by UV-laser ablation ICPMS. Journal of Analytical Atomic Spectrometry

Stoll, N. et al. (2023) Chemical and visual characterisation of EGRIP glacial ice and cloudy bands within. The Cryosphere

Stoll, N. et al. (2025) Linking crystallographic orientation and ice stream dynamics: evidence from the EastGRIP ice core. The Cryosphere

How to cite: Erhardt, T., Linda, M., Zeppenfeld, C., Weikusat, I., Fischer, H., and Müller, W.: Investigating the preservation of rapid climate signals in the ice matrix using 2D LA-ICP-MS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8223, https://doi.org/10.5194/egusphere-egu26-8223, 2026.

EGU26-8410 | ECS | Orals | CL1.2.7

Fidelity and stratigraphy of the Antarctic Allan Hills old ice archive from Continuous Flow Analysis 

Abigail Hudak, Asmita Banerjee, Christo Buizert, Edward Brook, Michael Kalk, Eric Steig, Lindsey Davidge, Andrew Schauer, Noah Brown, Liam Kirkpatrick, Jacob Chalif, Erich Osterberg, Miranda Miranda, Eric Saltzman, Valens Hishamunda, and John Higgins

Extending ice core records beyond 800 thousand years (kyr) is a pivotal goal in paleoclimate research. The Allan Hills Blue Ice Area, East Antarctica, provides a unique opportunity to meet this objective, with recent work recovering 6-million-year-old ice. The ice in this area demonstrates several peculiarities—such as strong layer thinning and folding—that warrant an in-depth investigation of its stratigraphy and the climate record it holds. Here, we present a high-resolution multi-measurement continuous flow analysis (CFA) on the upper 69 and 46 m from two shallow ice cores from the Allan Hills to evaluate these complexities.

Our CFA analysis measured methane, water stable isotopes, and particulate dust concentrations and size fractions, allowing us to characterize their variations and to assess the fidelity of the archive, i.e., how well environmental parameters are recorded and preserved in Allan Hills ice. We quantitatively compared the data structures of each climate element to the EPICA Dome C (EDC) climate record by evaluating the correlations and data distributions of each variable. Each climate parameter exhibits a narrower range of values than the EDC core, and distinct data distribution patterns that differed both between the Allan Hills cores and compared to EDC. The data revealed interglacial biases as evidenced by an overrepresentation of warmer climate states when compared to EDC. Discrete 40argon-dated sections from the two Allan Hills ice cores reveal age ranges from ~150-1200 kyr, with substantial age discontinuities and folding highlighting the complex stratigraphy of this ice. Our high-resolution investigation of this ice is a critical step toward better interpreting the discrete records from the Allan Hills, which extend beyond the 800 kyr continuous ice core record into the Pliocene, pushing our ice core records into unique and enigmatic parts of Earth’s climate history.

 

How to cite: Hudak, A., Banerjee, A., Buizert, C., Brook, E., Kalk, M., Steig, E., Davidge, L., Schauer, A., Brown, N., Kirkpatrick, L., Chalif, J., Osterberg, E., Miranda, M., Saltzman, E., Hishamunda, V., and Higgins, J.: Fidelity and stratigraphy of the Antarctic Allan Hills old ice archive from Continuous Flow Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8410, https://doi.org/10.5194/egusphere-egu26-8410, 2026.

EGU26-9377 | Posters on site | CL1.2.7

Gas extraction from CFA for 81Kr dating of the Beyond EPICA oldest ice 

Florian Ritterbusch, Jonas Wöhrl, Clara Baumbusch, David Wachs, Dieter Tetzner, Jack D. Humby, Shaun Miller, Elizabeth R. Thomas, Xin Feng, Jie Wang, Wei Jiang, Zheng-Tian Lu, Guo-Min Yang, Kerstin Urbach, Remi Dallmayr, Maria Hörhold, Johannes Freitag, Frank Wilhelms, Werner Aeschbach, and Pascal Bohleber

The Beyond EPICA oldest ice is a unique climate archive, continuously reaching back to possibly 1.5 Ma. The continuity of the signals in the ice core likely allows for developing a continuous timescale, mostly based on orbital tuning with O2/N2 and δ18Oatm. The obtained timescale can then be checked for consistency with marine records, 36Cl/10Be dating and possibly with magnetic tie points from cosmogenic isotopes. Since these consistency checks have caveats, additional absolute age constraints may prove useful.

The noble gas radioisotope 81Kr ( t1/2 = 229 ka ) with a dating range from 30 ka to 1.5 Ma can provide robust absolute age constraints in ice cores. Especially due to its gaseous and inert properties, its isotopic ratio is not altered by geochemical processes so that it preserves the pristine age information. 81Kr dating could provide additional absolute age constraints for the Beyond EPICA oldest ice. However, due to the high ice demand for numerous analyses on the core, there is no ice available for 81Kr analysis on discrete ice samples.

We present gas extraction from the Continuous Flow Analysis (CFA) of the Beyond EPICA oldest ice for 81Kr dating. The gas has been passively collected from the overflow of the debubbler into multi-layer aluminium-foil bags, which are routinely employed for 81Kr dating of groundwater. From the continuous melting of ~3 m long core, discrete ~100 mL STP gas samples have been extracted, and subsequently analyzed offline for 85Kr and 81Kr. Modern air contamination, likely from diffusion through the gas bags during storage, has been quantified with the anthropogenic 85Kr. The contamination can be avoided by transfer of the sampled gas from bag to metal container after collection. The 81Kr age constraints that could be obtained are consistent with preliminary timescales. The presented gas extraction method is non-invasive and requires minimum equipment, potentially providing a base for usage also in future CFA campaigns.

How to cite: Ritterbusch, F., Wöhrl, J., Baumbusch, C., Wachs, D., Tetzner, D., Humby, J. D., Miller, S., Thomas, E. R., Feng, X., Wang, J., Jiang, W., Lu, Z.-T., Yang, G.-M., Urbach, K., Dallmayr, R., Hörhold, M., Freitag, J., Wilhelms, F., Aeschbach, W., and Bohleber, P.: Gas extraction from CFA for 81Kr dating of the Beyond EPICA oldest ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9377, https://doi.org/10.5194/egusphere-egu26-9377, 2026.

EGU26-9646 | ECS | Posters on site | CL1.2.7

Is the penultimate deglaciation (Termination II) recorded in the folded ice in the deepest part of the Greenland NEEM ice core?   

Marie Bouchet, Anders Svensson, Amaëlle Landais, Elise Fourré, Thomas Blunier, Dorthe Dahl-Jensen, Julien Westhoff, Helle Astrid Kjær, Xin Feng, Wei Jiang, Qiao-Song Lin, Zheng-Tian Lu, Jie S. Wang, and Guo-Min Yang

The folded stratigraphy of the ice between 2432.2 and 2540 m in the Greenland NEEM ice core precludes direct access to climatic information older than 128.5 ka b2k (thousands of years before 2000 CE) (NEEM comm. Members, 2013). The disturbed stratigraphy is particularly unfortunate because this ice’s age corresponds to the Termination II (140–130 ka b2k). The climatic transition from the penultimate glacial period (MIS 6, 190–130 ka b2k) to the last interglacial (MIS 5e, 130–120 ka b2k) has not yet been extracted from Greenlandic ice core records.

In this study, we propose a possible reconstruction of the disturbed NEEM stratigraphy spanning the MIS 6–MIS 5e transition based on the succession of globally well-mixed gas parameters. The NEEM δ18Oice chronological sequence is obtained by comparing a new set of δ18O of atmospheric O2 and CH4 measurements from the bottom section of the NEEM core with their counterpart in composite Antarctic records. The proposed stratigraphy is also discussed with respect to three radiometric ages estimated from new 81Kr measurements from the bottom part of the NEEM core. The new gas measurements suggest that disturbed ice below 2432.2 m in the NEEM ice core contains, stratigraphically intact, but folded ice, with climatic information from MIS 6 and MIS 5e, possibly from the penultimate deglaciation, and that sections of MIS 5e are present twice in the ice. 

How to cite: Bouchet, M., Svensson, A., Landais, A., Fourré, E., Blunier, T., Dahl-Jensen, D., Westhoff, J., Kjær, H. A., Feng, X., Jiang, W., Lin, Q.-S., Lu, Z.-T., Wang, J. S., and Yang, G.-M.: Is the penultimate deglaciation (Termination II) recorded in the folded ice in the deepest part of the Greenland NEEM ice core?  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9646, https://doi.org/10.5194/egusphere-egu26-9646, 2026.

EGU26-9799 | ECS | Posters on site | CL1.2.7

Investigating the CH4 isotopic signature of debris rich basal ice: insight from Camp Century ice core.  

Lisa Ardoin, Carina Van der Veen, Saïda El Amari, Dorthe Dahl-Jensen, Jørgen Peder Steffensen, Jean-Louis Tison, Thomas Röckmann, and François Fripiat

Runoff waters at the margin of the Greenland Ice Sheet export CH₄-supersaturated waters originating from the ice-sheet bed, contributing to the global atmospheric CH₄ budget [1, 2]. This methane is of microbial origin, likely produced from a mixture of inorganic and ancient organic carbon buried beneath the ice sheet [1, 2, 3].

Debris-rich basal ice layers provide a unique opportunity to investigate the sources and sink of methane at the ice/bedrock interface. Previous studies have shown that Greenland debris-rich basal ice preserves large methane accumulations [4, 5, 6] and may represent a potential endmember contributing to CH4-rich meltwaters released during the melting season. At Camp Century, CH4 mixing ratios increase sharply from ~200 ppm to up to 30 000 ppm within 1 m above the ice/bed material transition [6]. Prokaryotic DNA analyses support the microbial origin, and indicate the presence of in situ methanotrophic communities, suggesting active CH4 consumption and oxidation to CO2 within the debris-rich ice [6].

Here, we present methane stable isotope measurements (δ13C-CH4 and δD-CH4) from 7 samples spanning this transition zone. Despite the large methane accumulation, debris-rich ice is strongly gas-depleted, and the limited sample size combined with high CH4 variability makes isotopic analyses technically challenging. CH4 was extracted using a melting-freeze extraction coupled to a cold-trap finger filled with HayeSep Q at Université Libre de Buxelles (ULB, Belgium) laboratory, allowing gases to be sealed in glass tubes to prevent atmospheric contamination. CH4 isotope analyses were performed at the Institute for Marine and Atmospheric Research Utrecht (IMAU, Netherlands) using a Thermo Delta Plus XP (δ13C and δD) [7].

The overall isotopic signature supports a microbial origin of CH4 via methanogenesis, consistent with GRIP values [4]. Despite substantial scatter in δ13C-CH4, a negative correlation is reported between CH4 concentration and both δ13C-CH4 and δD-CH4, consistent with preferential oxidation of lighter isotopes during methanotrophy. However, the observed relationship suggests a relatively low apparent fractionation factor compared to literature estimates. This could result from under-expression of the true isotope effect due to superimposed processes such as mixing or diffusion, or because the fractionation is intrinsically smaller under low-temperature conditions.

 

[1] Lamarche-Gagnon et al., 2019, Nature, 565(7737), 73-77. [2] Christiansen et al., 2021, Journal of Geophysical Research: Biogeosciences126(11), e2021JG006308. [3] Adnew et al., 2023, Geochimica et Cosmochimica Acta389, 249-264. [4] Souchez et al., 2006, Geophys. Res. Lett., 33, L24503. [5] Verbeke et al., 2002, Annals of Glaciology 35, 231-236. [6] Ardoin et al., submitted, The Cryosphere. [7] Menoud et al., 2020, Tellus B: Chemical and Physical Meteorology72(1), 1-20.

How to cite: Ardoin, L., Van der Veen, C., El Amari, S., Dahl-Jensen, D., Steffensen, J. P., Tison, J.-L., Röckmann, T., and Fripiat, F.: Investigating the CH4 isotopic signature of debris rich basal ice: insight from Camp Century ice core. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9799, https://doi.org/10.5194/egusphere-egu26-9799, 2026.

EGU26-10076 | ECS | Orals | CL1.2.7

On the link between Total Air Content (TAC) changes and local surface climate conditions in Greenland and Antarctica 

Héloïse Guilluy, Émilie Capron, Frédéric Parrenin, Vladimir Lipenkov, Jochen Schmitt, Zhipeng Wu, Qiuzhen Yin, Anna Klüssendorf, Amaëlle Landais, Patricia Martinerie, Barbara Seth, Hubertus Fischer, Roxanne Jacob, Grégory Teste, Thomas K. Bauska, Janani Venkatesh, and Dominique Raynaud

While air bubbles in polar ice cores preserve past atmospheric composition, the quantity of trapped air, known as Total Air Content (TAC), also carries significant paleoclimatic information. First applied to reconstruct past ice sheet elevation, TAC later became an orbital dating tool due to its correlation with local summer insolation. To address knowledge gaps and better understand TAC as an environmental proxy and as an orbital dating tool, we investigate the relationships between surface parameters, pore volume at close-off depth, and TAC changes at spatial and temporal scales.

We present and analyze a new dataset extending the EDC TAC record from 440 to 800 ka, as well as new TAC records from TALDICE and EDML covering the last glacial-interglacial cycle. We combine these new datasets with a compilation of published TAC data from deep and shallow ice cores across Antarctica and Greenland to explore the influence of surface climate parameters controlling the changes in TAC. Our spatial-scale analysis demonstrates that present-day TAC values relate primarily to atmospheric pressure and elevation. When examining pore volume at close-off (i.e. TAC values corrected for ideal gas law effects), we evidence a correlation with local half-year summer insolation for sites located in East Antarctica, suggesting a direct control of local insolation on firn densification in this region. Temporal-scale analyses on TAC records covering at least 45 ka confirm that TAC records contain an orbital-scale signature of local insolation but also show that local summer insolation alone cannot capture the full TAC variability. Multiple linear regression analyses incorporating both local insolation and reconstructed surface temperatures or accumulation better predict the observed TAC temporal changes, particularly during large glacial terminations. Our new EDC high-resolution record also reveals significant millennial-scale TAC changes during these glacial-interglacial transitions, highlighting that in addition to orbital-scale impacts of local summer insolation, millennial-to-multi-millennial-scale changes in surface climate parameters also influence temporal TAC changes. Our findings have implications for the use of TAC as an orbital dating tool as they suggest that performing an orbital tuning between TAC and local insolation without accounting for additional surface climate controls could introduce dating uncertainties of 1–4 ka. Building on these results, we present a new TAC profile measured on the Beyond EPICA Oldest Ice Core (BEOIC) core between 2438 and 2485 m depth and evaluate its potential for providing orbital age constraints on ice older than 800 ka and up to 1.2 million years.

How to cite: Guilluy, H., Capron, É., Parrenin, F., Lipenkov, V., Schmitt, J., Wu, Z., Yin, Q., Klüssendorf, A., Landais, A., Martinerie, P., Seth, B., Fischer, H., Jacob, R., Teste, G., Bauska, T. K., Venkatesh, J., and Raynaud, D.: On the link between Total Air Content (TAC) changes and local surface climate conditions in Greenland and Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10076, https://doi.org/10.5194/egusphere-egu26-10076, 2026.

EGU26-12002 | ECS | Orals | CL1.2.7

Dating an Amazonic ice core:disentangling a complex chemical record 

Manoela Brum Poitevin Portella, João Ilha, Elena Barbaro, Susan Kaspari, Carlo Barbante, Jefferson Simões, and Paul Mayewski

Ice cores are one of the best palaeoarchives for the most recent geological record. Their resolution is unmatched as it is possible to retrieve seasonal information of thousands of years of climatic archive. Therefore, dating is fundamental to interpreting these archives. Polar and temperate ice cores are well studied and have provided valuable records for paleoclimate interpretation. However, tropical ice cores remain under- studied because of many technical difficulties inherent to it, even though they have precious information on tropical climate dynamics. One of the biggest challenges is dating tropical ice cores. The relationship between ice depth and age is rarely straightforward and typically requires a multi-proxy approach - specially in tropical records, as they are not submitted to the typical polar and high-latitude climatic dynamic, due to its complex ice flow patterns, post-depositional processes like melting, and high background noise for chemical markers. Here we present results of a 128.3 m long ice core, collected from the Quelccaya Ice Cap, Peru (at 13°55’46,099”S, 70°49’21,557”W, 5.674 m above the sea level) during the austral winter of 2022. . In this study, we used refractory black carbon (rBC), ion concentration depth profiles and a series of frequency analysis to perform annual layer counting (manual and automated) based on seasonal variations. We try to assign to the dating reference horizons using volcanic signatures from historically known events and the El Niño Southern Oscillation (ENSO) index as tie points. The very low mobility of black carbon in ice and snowpack causes it to remain effectively locked in place after deposition, thereby creating a clear and consistent seasonal archive in the ice core data, with pronounced seasonality marked by peaks during the dry season (June – August). Ionic signal is less seasonal and presents intense remobilization indicating that the ice pack is rapidly losing part of its climatic signal that is so important for the understanding of tropical paleoclimate dynamics.
Keywords: ice core, Amazon, black carbon, paleoclimate

How to cite: Brum Poitevin Portella, M., Ilha, J., Barbaro, E., Kaspari, S., Barbante, C., Simões, J., and Mayewski, P.: Dating an Amazonic ice core:disentangling a complex chemical record, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12002, https://doi.org/10.5194/egusphere-egu26-12002, 2026.

EGU26-12071 | ECS | Posters on site | CL1.2.7

Centimeter-scale diffusion and in situ production effects on greenhouse gas records in the TALDICE ice core 

Lison Soussaintjean, Florian Krauss, Jochen Schmitt, Henrique Traeger, Thomas Bauska, and Hubertus Fischer

Ice cores provide the only direct archive of past atmospheric greenhouse gases (GHG). However, physical and chemical processes occurring before, during, and after bubble enclosure can alter the atmospheric signal recorded in ice. In particular, gas diffusion within the bubble-clathrate transition zone (BCTZ) has been shown to generate centimeter-scale, non-atmospheric variability, which we refer to as the “Lüthi effect” (Lüthi et al., 2010). Below the BCTZ, diffusive smoothing dampens these non-atmospheric signals but also atmospheric variability. While the Lüthi effect and diffusive smoothing have been documented for CO2 and the δO2/N2 ratio, their impact on N2O and CH4 remains poorly constrained. In addition, chemical reactions within the ice can alter atmospheric signals, particularly for N2O, which has been shown to be produced in situ by nitrate reduction in dust-rich Antarctic ice during glacial periods.

Here we investigate diffusion and in situ production processes potentially affecting CO2, CH4, and N2O by analyzing five samples from the BCTZ of the Talos Dome ice core (TALDICE). GHG concentrations were measured at centimeter-scale resolution using a novel laser sublimation extraction system coupled to a quantum cascade laser absorption spectrometer (Mächler et al., 2023). δO2/N2 ratios were analyzed by isotope ratio mass spectrometry following the recapture of the same samples after GHG measurements with the laser spectrometer.

Our results show for the first time that N2O and CH4 are also affected by the Lüthi effect in the BCTZ. The strong 1:1 correlation between CO2 and N2O variability suggests similar diffusion coefficients for these gases. These findings provide new constraints on N2O diffusion, relevant for modeling diffusive smoothing in deep and old ice such as the recently drilled Beyond EPICA ice core. Consistent with previous studies, our results indicate that the N2O record in TALDICE is not significantly affected by the aforementioned in situ production during glacial periods. The atmospheric N2O signal can therefore be retrieved when measurements are either spatially averaged to smooth the centimeter-scale variability induced by the Lüthi effect, obtained above the BCTZ, or taken well below the BCTZ where diffusive smoothing has attenuated this variability.

References

Lüthi, D., Bereiter, B., Stauffer, B., Winkler, R., Schwander, J., Kindler, P., Leuenberger, M., Kipfstuhl, S., Capron, E., Landais, A., Fischer, H., and Stocker, T. F.: CO2 and O2/N2 variations in and just below the bubble–clathrate transformation zone of Antarctic ice cores, Earth and Planetary Science Letters, 297, 226–233, https://doi.org/10.1016/j.epsl.2010.06.023, 2010.

Mächler, L., Baggenstos, D., Krauss, F., Schmitt, J., Bereiter, B., Walther, R., Reinhard, C., Tuzson, B., Emmenegger, L., and Fischer, H.: Laser-induced sublimation extraction for centimeter-resolution multi-species greenhouse gas analysis on ice cores, Atmos. Meas. Tech., 16, 355–372, https://doi.org/10.5194/amt-16-355-2023, 2023.

How to cite: Soussaintjean, L., Krauss, F., Schmitt, J., Traeger, H., Bauska, T., and Fischer, H.: Centimeter-scale diffusion and in situ production effects on greenhouse gas records in the TALDICE ice core, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12071, https://doi.org/10.5194/egusphere-egu26-12071, 2026.

EGU26-12832 | ECS | Orals | CL1.2.7

Raman non-destructive analysis of visible tephra layers in ice cores 

Marco Rabassi, Sergio Andò, Barbara Delmonte, Claudio Artoni, Deborah Fiorini, Elisa Malinverno, and Valter Maggi

Ice cores are exceptional archives of past climate variability, preserving forcing factors and proxies of the climate system’s response. Volcanic eruptions, when recorded as englacial tephra layers, provide insights into explosive volcanism, volcano–climate interactions, and enable long-range synchronization of paleoclimate records, provided the eruptive source is identified. Source attribution of far-travelled tephras requires geochemical characterisation of volcanic glass and comparison with known reference compositions. This task is complicated by the broad range of potential sources and the geochemical similarity of eruptive products. In this context, volcanic minerals, though less commonly used than glass, offer a valuable complementary tool for fingerprinting their source rocks.

More broadly, most analytical protocols rely on melting ice cores, compromising the preservation and future reuse of this important natural archive. As climate change poses increasing threat to global ice reserves, developing an innovative approach is critically needed.

Here, we present a novel, non-destructive Raman spectroscopy–based approach to analyse the mineralogy of visible tephra layers in ice cores. A tephra from Campbell Glacier, Antarctica (74°16′59″ S 164°10′52″ E), has been used to demonstrate advantages and pitfalls of this approach. The observed mineral assemblage is consistent with a strongly alkaline source and with its geochemical signature. This mineralogical dataset enables tephrochronological reconstructions and improves the precision and reliability of established analytical approaches for volcanic source fingerprinting.

How to cite: Rabassi, M., Andò, S., Delmonte, B., Artoni, C., Fiorini, D., Malinverno, E., and Maggi, V.: Raman non-destructive analysis of visible tephra layers in ice cores, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12832, https://doi.org/10.5194/egusphere-egu26-12832, 2026.

EGU26-13148 | ECS | Posters on site | CL1.2.7

PO14C dating of glacier ice – recent improvements for an easier device handling 

Johannes Wörner, Susanne Preunkert, and Werner Aeschbach

Over the last 15 years, studies of non-polar ice core archives have successfully demonstrated the usefulness of ice core dating via 14C in particular organic carbon (PO14C). It excels especially in deeper layers, where stratigraphic dating methods cannot be applied.
This presentation focuses on improvements made to the PO14C inline filtration-oxidation unit (REFILOX) system developed by Hoffmann et al. (2017, Radiocarbon, doi:10.1017/RDC.2017.99), which has been successfully applied in several Alpine ice core studies (e.g. Legrand et al. 2025, PNAS Nexus, doi:10.1093/pnasnexus/pgaf186).
The device was redesigned to allow an easier handling by avoiding the fragile, difficult to obtain and expensive quartz glass to stainless steel passages of the device. In addition, the material of the combustion chamber was changed to borosilicate glass, which is much easier to handle compared to quartz glass. Combined, these changes allow a faster and more thorough cleaning and assembly process. We introduce the new key characteristics of the modified setup, which already showed that the process blank could be maintained in the sub-microgram range. Beside blank characteristics and precision compared to standard material, a first application of the improved system is presented demonstrating its potential for radiocarbon dating of real glacier ice samples.

How to cite: Wörner, J., Preunkert, S., and Aeschbach, W.: PO14C dating of glacier ice – recent improvements for an easier device handling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13148, https://doi.org/10.5194/egusphere-egu26-13148, 2026.

EGU26-13352 | Orals | CL1.2.7

Ice-cores from temperate glaciers as paleoclimate archives in a warming world: what we know and what we need to know 

Giovanni Baccolo, Anja Eichler, Theo Jenk, Sandra Camara-Brugger, Michelle Worek, Francois Burgay, Barbara Delmonte, Clara Mangili, Valter Maggi, Elena Di Stefano, Pascal Bohleber, and Margit Schwikowski

Temperate glaciers have traditionally been viewed as unsuitable archives for paleoclimate and environmental reconstruction due to pervasive meltwater percolation and the consequent alteration or disruption of primary atmospheric signals. Yet, in the context of ongoing climate warming, many formerly cold accumulation glacier basins, traditionally targeted for ice-core drilling, are transitioning toward temperate conditions. Exploiting glaciers as sources of past environmental information will therefore increasingly require consideration of temperate glaciers worldwide.

We synthesize more than seven decades of temperate glacier ice-core research, from pioneering efforts in the 1950s to the recent developments. We discuss the physical and chemical mechanisms by which meltwater impacts ice stratigraphy and proxy records, including impurity elution, recrystallization, liquid water redistribution, and the fractionation of water stable isotopes. Through inter-site comparison across climatic regimes (tropical, mid-latitude and high-altitude temperate glaciers), we identify which proxies are most resilient to post-depositional modification and under which conditions meaningful environmental signals can be recovered.

Our results highlight that, while ice cores from temperate glaciers often lack the pristine stratigraphy of cold ice, they can still provide valuable records of climatic and environmental variability, particularly when interpreted in combination with meteorological observations, reanalysis products, and glaciological data.

With cold glaciers becoming increasingly scarce, in particular at low- and mid-latitudes, progress in ice-core science requires a better understanding of temperate ice processes. This contribution provides a reference framework from which future studies can build.

How to cite: Baccolo, G., Eichler, A., Jenk, T., Camara-Brugger, S., Worek, M., Burgay, F., Delmonte, B., Mangili, C., Maggi, V., Di Stefano, E., Bohleber, P., and Schwikowski, M.: Ice-cores from temperate glaciers as paleoclimate archives in a warming world: what we know and what we need to know, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13352, https://doi.org/10.5194/egusphere-egu26-13352, 2026.

EGU26-15040 | ECS | Posters on site | CL1.2.7

A Multiport CO₂ Extraction System for Accurate and Precise Measurements from Small Ice Core Samples 

Tyler Byland, Edward Brook, and Michael Kalk

Ice cores serve as valuable archives for past atmospheric conditions. They can provide direct records of past atmospheric CO₂ concentrations, but measurements from very old or stratigraphically disturbed ice are often limited by sample size and analytical precision. This study presents a custom-built multiport CO₂ extraction and crushing system designed to enable accurate and precise CO₂ concentration measurements from small ice samples (~10 g) with faster throughput than previous systems at OSU. The system allows sequential extraction of multiple samples under identical analytical conditions, improving throughput while minimizing contamination and analytical drift with ultimate throughput of 8-12 samples per day. 

We evaluate the performance of the multiport system through repeated analyses of ice standards and replicate small-sample measurements, assessing reproducibility, extraction efficiency, and measurement precision. CO₂ concentrations measured using this system demonstrate consistent reproducibility across ports, with precision comparable to previous methods at OSU. This method enables faster higher spatial resolution sampling and provides a foundation for improving CO₂ measurements in ancient ice where sample availability and potential respiratory inputs are key challenges.

How to cite: Byland, T., Brook, E., and Kalk, M.: A Multiport CO₂ Extraction System for Accurate and Precise Measurements from Small Ice Core Samples, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15040, https://doi.org/10.5194/egusphere-egu26-15040, 2026.

EGU26-15229 | Orals | CL1.2.7

Developing Hyperspectral Imaging Workflow for Ice Core Analysis 

Andrei Kurbatov, Roisin Rumsey, Sara Akiba, Hayley Beaudoin, Jennifer Schaefer, Daniel Breton, Edward Brook, Christo Buizert, John Fegyveresi, Tyler Fudge, Geoffrey Hargreaves, Curtis Labombard, Richard Nunn, Mark Royer, and Mikhail Zhizhin

Impurities trapped within glacial ice serve as unique archives of past environments. This study presents results from imaging ice core samples collected from Antarctica, Greenland, and the Arctic using the IceSpec (VNIR) hyperspectral imaging (HSI) system. Image processing algorithms, developed with open-source Python libraries (e.g., numpy, photutils, scikit-image, and SPy) enable the quantification of trapped air bubbles, dust content, and other impurities. This work expands parameterization of ice core physicochemical properties. 

HSI offers a robust, fast, high resolution and automated method that enhances traditional ice core analyses while introducing new capabilities. A key advantage is its non-destructive nature, which preserves full spectral information for subsequent impurity fingerprinting, chemical characterization and sample archiving.

This work was supported by National Science Foundation (NSF) grants 2149518 and 2149519, and by the Center for Oldest Ice Exploration (COLDEX), an NSF Science and Technology Center funded under grant NSF 2019719. We also acknowledge the logistical support provided by the NSF Antarctic Infrastructure and Logistics Program, the US Ice Drilling Program (supported by NSF Cooperative Agreement 1836328), the NSF Ice Core Facility, and the Antarctic Support Contractor.

How to cite: Kurbatov, A., Rumsey, R., Akiba, S., Beaudoin, H., Schaefer, J., Breton, D., Brook, E., Buizert, C., Fegyveresi, J., Fudge, T., Hargreaves, G., Labombard, C., Nunn, R., Royer, M., and Zhizhin, M.: Developing Hyperspectral Imaging Workflow for Ice Core Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15229, https://doi.org/10.5194/egusphere-egu26-15229, 2026.

EGU26-15278 | Orals | CL1.2.7

Photochemical Modification of Greenhouse Gas Concentrations in Antarctic Blue Ice 

Jinho Ahn, Giyoon Lee, Jaekyung Han, Sohee Lee, Syed Azharuddin, Ikumi Oyabu, Julia Peterson, Changhee Han, Motohiro Hirabayashi, Edward Brook, and Kenji Kawamura

We present evidence of greenhouse gases produced in-situ via photochemical reactions in Antarctic blue ice. Within near-surface layers (< 4.6 m), the air in bubbles exhibit markedly elevated concentrations of CO₂, CH₄, and N₂O. Considering the upward advection of the ice strata, these excess gas species are inferred to have originated within recent decades or the past century. Analytical evidences indicate that these excess greenhouse gases are products of photochemical reactions. The isotopic signatures of CO₂ and CH₄ elucidate that the carbon precursors are both organic and inorganic constituents embedded in the ice matrix.

To elucidate the kinetic pathways, we plan to perform laboratory simulations involving UV irradiation of ice samples, followed by rigorous analyses of the generated gas phases. Additionally, synthetic bubbly ice with precise gas compositions and specific ionic dopants, is being utilized to isolate the variables governing these reactions. We contend that occluded gas bubbles act as receptive vessels that preserve photochemical derivatives, thereby amplifying the detectability of minute chemical alterations. Our near future investigations will also address the isotopic fractionation dynamics occurring between the parent substrates and the resultant greenhouse gases.

How to cite: Ahn, J., Lee, G., Han, J., Lee, S., Azharuddin, S., Oyabu, I., Peterson, J., Han, C., Hirabayashi, M., Brook, E., and Kawamura, K.: Photochemical Modification of Greenhouse Gas Concentrations in Antarctic Blue Ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15278, https://doi.org/10.5194/egusphere-egu26-15278, 2026.

EGU26-15595 | Orals | CL1.2.7

81Kr Dating of 1 kg Polar Ice 

Xin Feng, Edward J Brook, Florian Ritterbusch, Guo-Min Yang, Jeffrey P Severinghaus, Jie S Wang, John A Higgins, Lei Zhao, Liang-Ting Sun, Matthew Harris, Michael L Bender, Nancy A.N. Bertler, Qiao-Song Lin, Sarah Shackleton, Taylor Ferrick, Wei Jiang, Ze-Hua Jia, and Zheng-Tian Lu

81Kr (t1/2 = 229 ka) is a valuable isotope for radiometric dating of water and ice with a dating range from thirty thousand to over one million years. Based on laser cooling and trapping, the detection method Atom Trap Trace Analysis (ATTA) has enabled 81Kr analysis at extremely low isotopic abundance levels in the environment. Here, we present the realization of a new-generation ATTA system that overcomes previous large sample-size requirements, making it possible to date polar ice-core samples of ~1 kg with ages up to 1.5 Ma.

We demonstrate the field applicability of this system through successful 81Kr dating of two dated 1-kg ice-core samples from Taylor Glacier, Antarctica. Based on this validation, we apply 81Kr dating to ancient ice samples with unknown ages from both polar regions. In Antarctica, we dated basal ice from the RICE core providing constraints for the existence of the Ross Ice Shelf through the Last Interglacial. In Greenland, we dated basal ice from the GISP2 ice core, obtaining 81Kr ages which implies that the central Greenland Ice Sheet persisted through the prolonged warm period of Marine Isotope Stage 11. To further reconstruct history and extent of the Greenland ice sheet, dating of ice core samples from other drill sites in Greenland is currently ongoing.

These examples demonstrate that the presented sample size reduction for 81Kr dating enables absolute age determination for stratigraphically disturbed basal ice, providing valuable information on the history of polar ice sheets.

How to cite: Feng, X., Brook, E. J., Ritterbusch, F., Yang, G.-M., Severinghaus, J. P., Wang, J. S., Higgins, J. A., Zhao, L., Sun, L.-T., Harris, M., Bender, M. L., Bertler, N. A. N., Lin, Q.-S., Shackleton, S., Ferrick, T., Jiang, W., Jia, Z.-H., and Lu, Z.-T.: 81Kr Dating of 1 kg Polar Ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15595, https://doi.org/10.5194/egusphere-egu26-15595, 2026.

EGU26-16803 | ECS | Orals | CL1.2.7

Drilling 613 m through Müller Ice Cap, Nunavut, Canada – Advances in drill equipment, innovations in camp infrastructure, first results from the ice core, and insights into the basal material beneath the ice 

Julien Westhoff, Alison Criscitiello, Bo Vinter, Grant Boeckmann, and Dorthe Dahl-Jensen and the the field, logistics, and ice core processing teams

From late March to late May 2025, a collaboration between Canada and Denmark drilled a 613-meter ice core through the Müller Ice Cap in the Canadian high Arctic. It is the deepest ice core in the Americas to date. The ice cap is in close proximity to the Arctic Ocean, supporting the primary goal of understanding the evolution of Arctic sea ice over the 10,000+ year record contained within the ice.

For the drilling, we utilized a newly designed intermediate winch and control system, combined with a previously existing tower, and the Danish deep drill system featuring 2.2 m core barrels. The newly designed winch is staged on a movable platform, resulting in a fixed level wind and a short distance to the tower.

Furthermore, we tested an inflatable tent to host the drilling and core processing. This worked well and withstood multiple days with strong winds and gusts above 40kt. The tent was a fraction of the weight of a traditional steel-framed tent.

Drilling concluded after 30 drilling days with 10m of debris-rich, silty ice by hitting bedrock at 612.98m depth. We drilled through numerous sandstones using carbide inserts on the ice core drill, and we recovered samples for optically stimulated luminescence dating.

The first results from the stable water isotopes (δ18O) and electric conductivity measurements (ECM) provide a profile over the full Holocene, as well as the transition from the Younger Dryas and Bølling-Allerød.

How to cite: Westhoff, J., Criscitiello, A., Vinter, B., Boeckmann, G., and Dahl-Jensen, D. and the the field, logistics, and ice core processing teams: Drilling 613 m through Müller Ice Cap, Nunavut, Canada – Advances in drill equipment, innovations in camp infrastructure, first results from the ice core, and insights into the basal material beneath the ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16803, https://doi.org/10.5194/egusphere-egu26-16803, 2026.

EGU26-17244 | ECS | Posters on site | CL1.2.7

Past and Recent Extreme Warm Events in Greenland derived from Firn Core Melt Layers 

Samira Zander, Maria Hörhold, Johannes Freitag, Ingo Sasgen, Sepp Kipfstuhl, Iben Koldtoft, Helle Astrid Kjaer, Chantal Zeppenfeld, Bo Vinther, and Thomas Laepple

Over the past few decades, the Greenland Ice Sheet has experienced multiple widespread surface melt events (e.g. 2012 and 2019), affecting nearly its entire surface. While seasonal surface melt occurs regularly at the margins of the Ice Sheet, it is rare in the high-elevation, central-north area and thus an indicator for extreme warm events. However, due to sparse in situ observations, particularly prior to the instrumental period little is known about the historical occurrence of such melt events.

Signatures of surface melt are archived within the firn column of the ice sheet as layers of refrozen melt water (melt layers), visually distinguishable from the surrounding unaffected firn and bubbly ice, due to the higher density and absence of air bubbles. We here analyse 22 firn cores from 15 sites across north-central Greenland, covering the past ~1000 years (until 2018 CE), to identify melt layers using visual inspection and micro-computed tomography. For the first time, we present a derived Greenland melt feature database, comprising over 1000 melt features.

Interpreting the melt features as a proxy for past extreme warm events allows to reconstruct the spatial extent and frequency of past melt events. Initial analyses indicate that both, elevation and geographic location strongly influence melt occurrence: lower-elevation sites experience more melt than higher-elevation sites, and the north-eastern basin shows more frequent surface melt than the north-western basin. This new dataset also places recent surface-melt events into a long-term context, demonstrating that the 2012 melt event was the most intense event in north-central Greenland over the last millennium.

How to cite: Zander, S., Hörhold, M., Freitag, J., Sasgen, I., Kipfstuhl, S., Koldtoft, I., Kjaer, H. A., Zeppenfeld, C., Vinther, B., and Laepple, T.: Past and Recent Extreme Warm Events in Greenland derived from Firn Core Melt Layers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17244, https://doi.org/10.5194/egusphere-egu26-17244, 2026.

EGU26-17427 | ECS | Posters on site | CL1.2.7

Unfolding reasons and consequences for the demise of the Greenland Ice Sheet: Perspective from biomarkers stored into basal ice 

Mathia Sabino, Alfredo Martínez-García, Florian Rubach, Mareike Schmitt, Petra Vinšová, Arthur François Tanguy Fouillé, Charlotte Prud’Homme, Marek Stibal, Sophie Opfergelt, Anders Svensson, Dorthe Dahl-Jensen, Pierre-Henri Blard, Jean-Louis Tison, and François Fripiat

Ice cores retrieved over the past 50 years from the Greenland Ice Sheet archive invaluable clues about the response of large ice caps to global climate dynamics. Evidence indicates that during past warm interglacial periods, the Greenland Ice Sheet likely experienced significant retreat and may even have collapsed entirely. However, the factors controlling the stability of the Greenland Ice Sheet, its origin, and the environmental implications of its demise are still scarcely understood.

Basal ice, namely debris-rich ice found at the base of the ice mass near the substrate, has the highest potential to preserve information that may help constrain climate conditions conducive to the demise of an ice sheet. To contribute to unfolding these precious archives, we aim to develop and apply innovative organic geochemical techniques targeting fossil organic molecules that can be used as biological markers (in short, biomarkers) for the ecosystems that could have been entrained at the base of the Greenland Ice Sheet during its formation.

Here, we show preliminary results on the methodology developed, including tests on artificial and natural basal ice samples. We also performed geochemical analyses on material (river sediments and permafrost soils) collected from a modern periglacial environment during an expedition to the western margin of the Greenland Ice Sheet. The comparison with the organic geochemical fingerprint preserved in basal material retrieved in deep ice core drilling will help us to reconstruct past ecosystems and ultimately gain insights into the climate and environmental conditions that existed prior to the buildup of the Greenland Ice Sheet.

How to cite: Sabino, M., Martínez-García, A., Rubach, F., Schmitt, M., Vinšová, P., Fouillé, A. F. T., Prud’Homme, C., Stibal, M., Opfergelt, S., Svensson, A., Dahl-Jensen, D., Blard, P.-H., Tison, J.-L., and Fripiat, F.: Unfolding reasons and consequences for the demise of the Greenland Ice Sheet: Perspective from biomarkers stored into basal ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17427, https://doi.org/10.5194/egusphere-egu26-17427, 2026.

EGU26-17690 | ECS | Posters on site | CL1.2.7

A Filtered View of Time: Improving the performance of the 36Cl / 10Be chronometer in Greenland ice cores by separation of the 10Be budget in ice and dust 

Jonathan Adams, Marie Protin, Raimund Muscheler, Elise Fourre, Thomas Combacal, Dorthe Dahl-Jensen, Jørgen Peder Steffensen, Anders Svensson, Francois Fripiat, Aster Team, Eidgenössische Technische Hochschule Zürich Team, and Pierre-Henri Blard

Absolute dating methods are required to provide accurate age estimates of extremely thinned and folded layers in the deepest sections of ice cores. The 36Cl / 10Be chronometer works on the principle that the ratio of 36Cl (half-life; 301 kyr) will decrease relative to 10Be (half-life; 1.4 Myr) with increasing age of ice. This method is especially desirable because it generally requires less ice for analysis than other absolute dating techniques such as 81Kr. However, both 36Cl and 10Be are affected by processes that complicate their reliability as geochronological tools. For instance, at low accumulation sites, the 36Cl inventory can be depleted through hydrogen chloride outgassing, however 36Cl is largely preserved in glacial periods due to increased buffering from alkaline species associated with increased dust content. Conversely, increased dust content during glacial periods can complicate the 10Be inventory due to adsorption of  10Be onto dust. In deep ice, such 10Be migration has resulted in observations of the 10Be concentration decreasing faster than expected from physical decay alone (Kappelt et al., 2025), which can lead to potential age underestimates when using the 36Cl / 10Be chronometer.

 

Here we focus on the issue of 10Be migration in deep ice by using a 0.45μm filter to separate the 10Be inventory attached to dust particles and in ice prior to 10Be measurement. We present preliminary results using our filtration method on Holocene, LGM and MIS-4 samples from the Dye-3 ice core from southern Greenland. Our results confirm that the impact of dust on the 10Be budget is more pronounced during glacial periods. Additionally, we use our filtration technique to test its potential to resolve the depletion of 10Be observed in the deeper sections of ice cores, by working on deep core sections that are independently dated by 81Kr. To make progress on better constraining the 10Be signal, we also present a modified sequential leaching technique, previously applied to ocean and river sediments. By performing sequential leaching on the filtered dust, we aim to separate the labile meteoric 10Be fraction (adsorbed from the ice) from the meteoric 10Be fraction that was already present at the dust surface prior to the incorporation of the dust into the ice. In better constraining the impact of 10Be migration onto dust on the total 10Be inventory in deep ice cores we hope to improve the accuracy of the paired 36Cl / 10Be chronometer for small-sample (< 1 kg) ice core analyses.

How to cite: Adams, J., Protin, M., Muscheler, R., Fourre, E., Combacal, T., Dahl-Jensen, D., Steffensen, J. P., Svensson, A., Fripiat, F., Team, A., Team, E. T. H. Z., and Blard, P.-H.: A Filtered View of Time: Improving the performance of the 36Cl / 10Be chronometer in Greenland ice cores by separation of the 10Be budget in ice and dust, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17690, https://doi.org/10.5194/egusphere-egu26-17690, 2026.

EGU26-18172 | ECS | Posters on site | CL1.2.7

Aerosol data from the EGRIP ice core covering the Last Glacial Maximum 

Chantal Zeppenfeld, Sarah Jackson, Geunwoo Lee, Tobias Erhardt, Helle Astrid Kjær, Camilla Marie Jensen, and Hubertus Fischer

Polar ice cores are archives of past climate conditions and atmospheric composition. Atmospheric aerosols deposited on the ice sheets and subsequently preserved in the ice provide detailed records of past atmospheric conditions. Analyses of these impurities therefore offer valuable insights into environmental changes in the past.

Here we present high-resolution impurity records from the East Greenland Ice Core Project (EGRIP) ice core measured with the University of Bern continuous flow analysis (CFA) set-up. Continuous melting and the analysis of only the inner part of the ice stick allows for high resolution while minimizing contamination. The analyzed components include water-insoluble dust particles as well as the dissolved impurities calcium, ammonium, and nitrate. For the dust record, we focus on the previously not studied changes in the main mode of the dust number concentration (<1 µm) and the dust refractive index. The dissolved species act as proxies for aridity (calcium) as well as vegetation cover and biomass burning (ammonium). Additionally, volcanic eruptions are imprinted in the electrolytic conductivity record of the meltwater.

The records span the period from 30k to 15k years BP, covering the Last Glacial Maximum (LGM). In Greenland ice cores, the LGM is characterized by high impurity content including dust, calcium, and nitrate. In contrast, ammonium concentrations are consistently low, reflecting extensive northern hemisphere ice sheets during this period. We observe dust concentrations up to 60 times higher than during the Holocene for particles in the 0.2-2 µm size range. Although dust concentrations remain high throughout the studied period, they exhibit pronounced variability. While the refractive index stays largely constant, the dust size distribution varies, but not in parallel with the concentration. Since the preserved size distribution is primarily controlled by atmospheric transport time, we hypothesize that dust source region contributions to Greenland changed during the LGM.

How to cite: Zeppenfeld, C., Jackson, S., Lee, G., Erhardt, T., Kjær, H. A., Jensen, C. M., and Fischer, H.: Aerosol data from the EGRIP ice core covering the Last Glacial Maximum, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18172, https://doi.org/10.5194/egusphere-egu26-18172, 2026.

EGU26-19191 * | ECS | Orals | CL1.2.7 | Highlight

39Ar and 14C on ice - Dating the remainders of Alpine glaciers amid rapid mass loss 

David Wachs, Azzurra Spagnesi, Pascal Bohleber, Andrea Fischer, Martin Stocker-Waldhuber, Alexander Junkermann, Niclas Mandaric, Florian Meienburg, Theo Jenk, Markus Oberthaler, and Werner Aeschbach

In the wake of a warming global climate, prolonged periods of negative mass balance affect even high-altitude Alpine glaciers. For these ideal candidates for paleoclimate-related ice core studies, this greatly complicates the already challenging task of establishing an age-depth relationship, because both the age at depth and at the surface is unknown. Radiometric ice dating methods are an important key to overcome this challenge. For Alpine glaciers that have already lost significant amounts of surface ice, the combined use of the radiometric tracers 39Ar and 14C has proven to be particularly effective (Legrand et al., 2025, Hou et al., 2025, Wachs et al., 2026).
Among other applications, we will present a recently published (Wachs et al., 2026) study on the age-depth profile of the summit glacier of Weißseespitze (WSS, 3500 m a.s.l.) in the Austrian Alps. All 39Ar samples were measured using atom trap trace analysis (ATTA), while 14C data from an earlier publication (Bohleber et al., 2020) complete the record. Constrained by the measurements, age modeling using least squares fitting and Monte Carlo sampling was performed to find a suitable glaciological model and to establish a continuous age-depth relationship.
The results show that the surface ice at WSS dates back approximately 400 years, emphasizing the extent of recent ice loss. At the same time, the continuous age-depth relationship shows no evidence of prolonged periods of mass loss at WSS within the 6000 years glaciation history prior to the present. The resulting age–depth relationship thus forms the basis for the historical interpretation of chemical records from WSS, such as recently published by Spagnesi et al., 2026, and their intercomparison with other paleoclimate archives.
Beyond WSS, the combined 39Ar-14C dating approach is readily transferable to other vulnerable Alpine ice archives. We will discuss ongoing work at sites such as Jamtalferner and others and illustrate its potential to establish robust chronologies across a range of Alpine glacial settings.

Bohleber et al., New glacier evidence for ice-free summits during the life of the Tyrolean Iceman, Scientific Reports, 2020

Hou et al., A radiometric timescale challenges the chronology of the iconic 1992 Guliya ice core, Science Advances, 2025

Legrand et al., Alpine ice core record of large changes in dust, sea-salt, and biogenic aerosol over Europe during deglaciation, PNAS Nexus, 2025

Spagnesi et al., New chemical signatures from Weißseespitze ice cores (Eastern Alps): pre-industrial pollution traces from Roman Empire to Early Modern Period, Frontiers in Earth Science, 2026

Wachs et al., A continuous 6000 year age depth relationship for the remainder of the Weißseespitze summit glacier based on 39Ar and 14C dating, Climate of the Past, 2026

How to cite: Wachs, D., Spagnesi, A., Bohleber, P., Fischer, A., Stocker-Waldhuber, M., Junkermann, A., Mandaric, N., Meienburg, F., Jenk, T., Oberthaler, M., and Aeschbach, W.: 39Ar and 14C on ice - Dating the remainders of Alpine glaciers amid rapid mass loss, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19191, https://doi.org/10.5194/egusphere-egu26-19191, 2026.

EGU26-19279 | ECS | Posters on site | CL1.2.7

BURNice: Global biomass burning reconstruction using ethane in polar ice cores 

Jennifer Campos Ayala, Markus Grimmer, Barbara Seth, Florian Krauss, Jochen Schmitt, Christoph C. Raible, Daphne Meidan, Alfonso Saiz-Lopez, and Hubertus Fischer

The BURNice project aims to quantify global fire emissions during important climate events from the Holocene to the last interglacial termination using ethane in polar ice cores. The project aims to combine analytical measurements and model simulations to explore the fate of ethane (C2H6) in the atmosphere in the past. Ethane is a short-lived non-methane hydrocarbon with a simple atmospheric budget. Ethane is primarily emitted into the atmosphere by fire and is removed via reaction with OH and Cl radicals, resulting in a lifetime of ~2 months.

Measurements of ethane in ice cores are conducted using continuous sublimation extraction (CSE) method in tandem with GC-IRMS for parallel quantification of ethane, methane (CH4), methane isotopes (δ13CH4), and other trace gases. We perform simulations using the Community Earth System Model (CESM) with an improved representation of halogen chemistry to investigate the spatio-temporal dynamics of ethane in the paleo-atmosphere. Preliminary results focus on the effect of the Cl-sink on ethane in modern-day, which is poorly constrained.

This study presents 1) advancements in measurements of ethane in NH and SH ice cores using CSE-GC-IRMS, and 2) results of sink-varied modern-day simulations of ethane in the atmosphere using CESM.

How to cite: Campos Ayala, J., Grimmer, M., Seth, B., Krauss, F., Schmitt, J., Raible, C. C., Meidan, D., Saiz-Lopez, A., and Fischer, H.: BURNice: Global biomass burning reconstruction using ethane in polar ice cores, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19279, https://doi.org/10.5194/egusphere-egu26-19279, 2026.

EGU26-19939 | ECS | Posters on site | CL1.2.7

Microbial Analyses of a Pre-Industrial Ice Core from Weißseespitze, Tyrol 

Svenja Conzelmann, Birgit Sattler, Lea Hartl, Andrea Fischer, Daniel Gattinger, Monika Summerer, Alessandro Sergio Cuzzeri, Martin Stocker-Waldhuber, Bernd Seiser, Anne Hartig, Giulia Bertolotti, and Andreas Gschwentner

Ice cores represent valuable archives of past climatic, chemical, and biological conditions. Beyond their role in paleoclimate reconstruction, alpine ice cores enable the investigation of microbial biodiversity in extreme frozen environments and natural baselines of antibiotic resistance. This study analyses an alpine ice core from Weißseespitze (Ötztal Alps, Tyrol, Austria) (46°50’46.61393"N, 10°43’00.42181"E) to assess depth-dependent changes in bacterial and fungal communities and antibiotic resistance traits of bacteria.

The ice core was extracted in June 2025 using thermal drilling. It was 5.42 m long and covers a period from ~450–480 years before present at the surface to ~6000 years before present at the base. As a cold-based ice cap, the Weißseespitze is a suitable and well established study site in the Eastern Alps for ice core research. Until now, research has focused on gathering physical and chemical data; therefore, this study aims to provide the first biological information.

The biodiversity of bacteria is evaluated via 16S rRNA gene sequencing using the primers 16S-V3/4 and full-length 16S, while fungal biodiversity is evaluated with ITS regions using the ITS_Fung primer. Nanopore sequencing is used for both assessments. Antibiotic resistance is investigated using a cultivation-based strategy with a disk diffusion test at 20°C and 4°C. The antibiotics tested are of natural, semi-synthetic, and synthetic origin. Subsequently, selected resistant isolates are analysed genetically. 

First results of this study showed a low amount of DNA in the samples. It has also already been demonstrated that bacterial cell abundance varies along the depth profile, as do dissolved organic carbon (DOC) concentrations. In general, we hypothesize that microbial community composition and antibiotic resistance traits vary with depth in response to changes in ice structure, depositional processes, and climatic conditions, while upper layers may additionally reflect anthropogenic influence. This study contributes to a better understanding of microbial persistence in cryospheric environments, natural reservoirs of antibiotic resistance, and potential implications for downstream ecosystems and astrobiological research.

How to cite: Conzelmann, S., Sattler, B., Hartl, L., Fischer, A., Gattinger, D., Summerer, M., Cuzzeri, A. S., Stocker-Waldhuber, M., Seiser, B., Hartig, A., Bertolotti, G., and Gschwentner, A.: Microbial Analyses of a Pre-Industrial Ice Core from Weißseespitze, Tyrol, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19939, https://doi.org/10.5194/egusphere-egu26-19939, 2026.

EGU26-21792 | Orals | CL1.2.7

An overview of the layered structure of the polar ice sheet based on crystalline textural properties of the Dome Fuji summit ice core, Antarctica 

Shuji Fujita, Tomotaka Saruya, Atsushi Miyamoto, Kumiko Goto-Azuma, Motohiro Hirabayashi, Akira Hori, Yoshinori Iizuka, Takao Kameda, Hiroshi Ohno, Wataru Shigeyama, and Shun Tsutaki

This study provides an overview of the layered structure of Antarctic ice sheets, focusing on the crystalline textural properties and deformational regimes in the Dome Fuji ice core. Polar ice sheets consist of layers with diverse rheological characteristics, shaped by depositional processes such as atmospheric aerosol deposition. Layer thickness varies from millimeters (annual layers) to thicknesses spanning glacial-interglacial periods, with the initial ice fabric forming during firnification.

Key factors influencing the rheology of ice include ion content (e.g., Cl−, F−, NH4+) and insoluble particles such as salts and dust. Ions can substitute within the ice crystal lattice, affecting dislocation density, viscosity, and deformation behavior. These influences persist from firnification to the basal layers of the ice sheet. Notably, salt inclusions have larger volume fractions than dust particles, significantly impacting microstructure evolution.

The ice sheet’s deformation can be divided into two regimes: the upper 80% of the ice sheet, characterized by lower strain and temperature gradients, and the lower 20%, where higher temperatures and strain induce complex recrystallization processes. Four primary factors drive the evolution of crystal orientation fabrics and microstructures: (i) temperature conditions, (ii) strain configurations, (iii) insoluble particle effects, and (iv) dynamic recrystallization, including grain boundary migration and the formation of new grains. These processes result in a deformational history unique to each layer, spanning up to one million years.

Understanding these layered structures has significant implications. For ice sheet modeling, they provide constraints on strain values and inform models of vertical thinning. For ice core sciences, the layered structure highlights the importance of drilling sites. Dome summit sites preserve continuous, undisturbed records of ancient ice, while locations away from domes risk basal disturbances, including folding, faulting, and layer mixing.

This research enhances our understanding of ice sheet dynamics and supports the development of improved dating models, contributing to studies of Earth's climate history over millennia.

 

How to cite: Fujita, S., Saruya, T., Miyamoto, A., Goto-Azuma, K., Hirabayashi, M., Hori, A., Iizuka, Y., Kameda, T., Ohno, H., Shigeyama, W., and Tsutaki, S.: An overview of the layered structure of the polar ice sheet based on crystalline textural properties of the Dome Fuji summit ice core, Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21792, https://doi.org/10.5194/egusphere-egu26-21792, 2026.

EGU26-4244 | Orals | CL1.2.8

Dust Concentration and grain size record from the Beyond EPICA oldest ice: implications for dust preservation in the oldest sections of the core. 

Barbara Delmonte, Elena Di Stefano, Hubertus Fischer, Sarah Jackson, Luca Lanci, Geunwoo Lee, and Marco Rabassi

Mineral dust concentration and grain size preserved in polar ice cores serve as critical paleoclimate proxies spanning the Holocene and Pleistocene epochs. These parameters yield valuable information about past environmental conditions in dust source regions, atmospheric dust loading and transport dynamics, exhibiting pronounced variability across glacial–interglacial cycles. The Antarctic dust deposition record derived from the ∼800.000 years old EPICA Dome C (EDC) ice core has now been extended further back into the Early Pleistocene through analysis of the Beyond EPICA-Oldest Ice Core (BEOIC). Here we present the preliminary Coulter Counter-derived dust concentration (0.6-18 μm range) and volume-size data from BEOIC for the period predating the EDC record, and compare them with available marine dust records. Dust concentration and grain size variability in the oldest ice enable the identification of glacial and interglacial periods, with characteristic size distributions showing relatively coarser particles during interglacials and finer particles during glacials.

The use of aeolian dust as a paleoclimatic proxy in ice cores assumes that englacial processes preserve the original physical and chemical signals. However, this paradigm has been partially challenged by evidence of in situ alteration processes that induce physical and geochemical (including mineralogical) modifications within the ice. The extent and nature of these processes in the BEOIC are currently under investigation. Preliminary observations are presented and compared with findings from other Antarctic ice cores (TALDICE, RICE) to evaluate the reliability of paleoclimatic signal preservation in the oldest ice sections.

How to cite: Delmonte, B., Di Stefano, E., Fischer, H., Jackson, S., Lanci, L., Lee, G., and Rabassi, M.: Dust Concentration and grain size record from the Beyond EPICA oldest ice: implications for dust preservation in the oldest sections of the core., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4244, https://doi.org/10.5194/egusphere-egu26-4244, 2026.

EGU26-4844 | ECS | Posters on site | CL1.2.8

Millennial scale resolution Mean Ocean Temperature over the MIS 9 glacial inception 

Henrique Traeger, Markus Grimmer, Patrice Tinner, Jochen Schmitt, and Hubertus Fischer

The two major heat reservoirs on the Earth’s surface are oceans and the latent heat required to melt glaciers and ice sheets. Of these, the ocean is the largest and the fluctuations in Ocean Heat Content (OHC) therefore yield insights into Earth’s energy balance through time. We reconstruct OHC fluctuations through Mean Ocean Temperature (MOT) change, in turn reconstructed through the measurement of noble gas ratios in ice cores. Noble gases are inert; on the Earth’s surface they mainly partition between the atmosphere and the oceans depending on the latter’s temperature. From ice core measurements, past atmospheric noble gas ratios can be determined and from these a global, integrated, mean ocean temperature record is obtained. Until recently, MOT reconstructions were mostly focused on glacial Terminations, leaving the sections separating them sparsely covered.

Here, we present a millennial scale resolution MOT reconstruction for the MIS 9 glacial inception. The MIS 9e overshoot (centred around 336 kyrs) sees an intermittent 2°C MOT rise before returning to interglacial values. During the glacial inception itself (~325 – 307 kyrs), the oceans cooled by approximately 2°C, roughly two thirds of the glacial period’s total. This initial MOT drop coincides with a decline in both Southern Ocean and Antarctic plateau temperatures. However, we note a decoupling between decreasing temperatures and CO2 concentration; the latter plateaus for around five millennia after the start of ocean temperature decline. Further MOT measurements are planned on the Beyond EPICA ice core covering the most recent glacial inception (104-126 kyrs). These could lead to additional insights into glacial inceptions.

How to cite: Traeger, H., Grimmer, M., Tinner, P., Schmitt, J., and Fischer, H.: Millennial scale resolution Mean Ocean Temperature over the MIS 9 glacial inception, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4844, https://doi.org/10.5194/egusphere-egu26-4844, 2026.

EGU26-5446 | Posters on site | CL1.2.8

High resolution water isotopic records on the Little Dome C firn cores and Beyond EPICA ice core for past climate and atmospheric water cycle reconstructions 

Bénédicte Minster, Emma Samin, Amaëlle Landais, Elise Fourré, Mathieu Casado, Adrien Ooms, Niels Dutrievoz, Cécile Agosta, Valérie Masson-Delmotte, Thomas Combacal, Barbara Stenni, Matteo Salvini, Maria Hörhold, Frank Wilhelms, Melanie Behrens, Johannes Freigtag, Daniela Jansen, Ilka Weikusat, Hans Christian Steen-Larsen, and Vasileios Gkinis and the The Beyond Epica water isotopes consortium

Water stable isotope records from Antarctic ice cores provide exceptional paleoclimatic information, currently spanning the last 800,000 years from the EPICA Dome C ice core (EDC). The recently retrieved Beyond EPICA Little Dome C (BELDC) ice cores should enable us to extend continuous Antarctica paleoclimate records back to at least 1.2 or even 1.5 million years ago, document past Antarctic climate and water cycle variability, and compare these new records with information extracted from other paleoclimatic archives.

The quantification of reliable past climate information based on high resolution water isotope records in deep Antarctic ice cores requires to characterize post-deposition processes which alter the initial precipitation isotopic composition. The isotopic composition of surface snow is affected by processes such as sublimation, hoar formation and snow redeposition. Then, diffusion smoothes isotopic profiles both in the firn and in the ice. Such processes can be particularly important in very low accumulation sites such as Little Dome C, and for very old ice.

For this purpose, we explore insights from new high-resolution measurements of δ18O of water from recent Little Dome C (LDC) firn cores and BELDC ice core, with a focus on three specific time slices.

First, we present the δ18O continuous flow analysis over the top 84 m of the LDC firn, spanning the past 2154 years based on volcanic age markers. This allows to estimate the LDC accumulation rate at approximately 24 mmwe.yr-1.  Our record is confronted to series generated by a virtual firn core model. Surface mixing plays an important role in reshaping the recorded signal within the first 3 m, with a best agreement obtained with an 8 cm mixing layer. Our results highlight that the diffusion is overestimated based on classical diffusion modelling.

We then focus on the last interglacial period, MIS5, and compare 2.5 and 10 cm dD resolution measurements from BELDC with earlier 11 cm records from EPICA Dome C, where the highest δD anomaly of the last 800 ka is observed.

Finally, we present 2.5 cm resolution δD records from BELDC spanning the time period prior to the EPICA Dome C record, from MIS23 (around 900 ka) to warm MIS31(around 1.08 to 1 Ma).

How to cite: Minster, B., Samin, E., Landais, A., Fourré, E., Casado, M., Ooms, A., Dutrievoz, N., Agosta, C., Masson-Delmotte, V., Combacal, T., Stenni, B., Salvini, M., Hörhold, M., Wilhelms, F., Behrens, M., Freigtag, J., Jansen, D., Weikusat, I., Steen-Larsen, H. C., and Gkinis, V. and the The Beyond Epica water isotopes consortium: High resolution water isotopic records on the Little Dome C firn cores and Beyond EPICA ice core for past climate and atmospheric water cycle reconstructions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5446, https://doi.org/10.5194/egusphere-egu26-5446, 2026.

EGU26-5532 | ECS | Orals | CL1.2.8

Evaluating Signal Attenuation and Gas Diffusion Impacts on Orbital Dating and Atmospheric Evolution of O2 Concentration in the Beyond EPICA Ice Core 

Anna Klüssendorf, Louisa Brückner, Mathieu Casado, Elodie Brugère, Léa Baubant, Frédéric Prié, Elise Fourré, Thomas Combacal, and Amaëlle Landais and the Beyond EPICA Community

Polar ice cores provide valuable insights into past environmental and climatic variability. The recently drilled Beyond EPICA ice core is believed to preserve the climate history of the past 1.5 million years (Ma). To effectively interpret the climatic information retrieved from this ice core, it is imperative to establish a precise chronology, assigning an age to each individual depth level. Dating old ice strongly relies on orbital tuning of the isotopic and elemental composition of atmospheric oxygen and nitrogen, extracted from air bubbles enclosed within the ice to variations in solar insolation. However, extensive layer thinning and enhanced vertical gas diffusion in the deep section of an ice core can substantially impact the signal preservation of these dating tools. Recently obtained data of δ18O of atmospheric O218Oatm) from the deepest 100 metres, possibly spanning from ~0.7 to 1.5 Ma, reveal a significant attenuation of the orbital signal amplitude prior to 1.1 Ma, challenging precise orbital dating. Diffusion effects however does not impede reconstruction of the long-term trend in O2 atmospheric concentration and isotopic composition. While δ18Oatm remains stable throughout this period, the relative concentration of atmospheric O2 distinctly decreases around 0.9 Ma. Although this long-term trend with time aligns with previous observations during more recent periods, the natural variation of O2 concentration in the atmosphere potentially poses an additional difficulty for orbital dating accuracy in which the δ(O2/N2) orbital signal is driven by local insolation. We propose using δ(Ar/N2) as a supplementary dating tool, as this ratio exhibits a similar relationship with local insolation while being independent of oxygen. Further, the new deep Beyond EPICA δ(Ar/N2) record reveals a higher signal amplitude in the deepest section compared to δ(O2/N2) because Ar is expected to diffuse less than O2, thereby enhancing the potential for orbital dating. Thus, integrating atmospheric δ18O, δ(O2/N2), and δ(Ar/N2) can facilitate to establish a chronology for the Beyond EPICA ice core, provided that high-precision and high-resolution data are ensured.

 

 

How to cite: Klüssendorf, A., Brückner, L., Casado, M., Brugère, E., Baubant, L., Prié, F., Fourré, E., Combacal, T., and Landais, A. and the Beyond EPICA Community: Evaluating Signal Attenuation and Gas Diffusion Impacts on Orbital Dating and Atmospheric Evolution of O2 Concentration in the Beyond EPICA Ice Core, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5532, https://doi.org/10.5194/egusphere-egu26-5532, 2026.

EGU26-5685 | ECS | Posters on site | CL1.2.8

The Beyond EPICA Oldest Ice Impurities Continuous Flow Analysis 

Jack Humby and Elizabeth Thomas and the Beyond EPICA Oldest Ice Core Impurities CFA Team

We present an optimised impurities continuous-flow analysis (CFA) method specifically developed to analyse the Beyond EPICA Oldest Ice Core (BE-OIC; >700 ky bp). Hosted at the British Antarctic Survey (BAS1) and operated collaboratively with our BE-OI partners2-12, the new CFA method was designed to operate at a melt rate of 1.5 cm min-1. The system included the continuous analyses of trace elements (triple quadrupole inductively-coupled plasma mass spectrometry, Agilent 8900 ICP-QQQ-MS/MS & inductively-coupled plasma optical emission spectroscopy, Agilent 5900 ICP-OES; BAS1); major anions (Cl-, SO42-, NO3- and MSA, Dionex fast ion chromatography, FIC; BAS1); NH4+ (fluorometry; BAS1); electrolytic conductivity (Dionex CDM-1 & Amber Science ECM 3201; BAS1); insoluble particulate size distribution (Abakus Klotz laser diffraction spectrometry, and EOS Single Particle Extinction Scattering, SPES2; U. Bern2); and stable water isotopes (δ18O, δ2H; Picarro cavity ring-down spectrometry, CRDS; U. Bern2, BE-OI Isotope Consortium7-10,12). For the first time, we present sections of BE-OIC chemistry data, focusing on trace elements (ICP-QQQ-MS & ICP-OES) and major anions (FIC). 
In addition, the CFA campaign provided discrete liquid samples for single-particle trace elemental analysis (U. Bern2), organic analysis (U. Cambridge3, Ca’ Foscari U. Venice9&CNR-ISP10), δ34S (U. St. Andrews5), diatoms (BAS1), halogens (Ca’ Foscari U. Venice9 & CNR-ISP10), and tephra (BAS1, U. St. Andrews5 & Swansea U.6). Furthermore, discrete gas samples were collected for 81Kr dating (Heidelberg U.11). 

How to cite: Humby, J. and Thomas, E. and the Beyond EPICA Oldest Ice Core Impurities CFA Team: The Beyond EPICA Oldest Ice Impurities Continuous Flow Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5685, https://doi.org/10.5194/egusphere-egu26-5685, 2026.

EGU26-5716 | ECS | Posters on site | CL1.2.8

First Δ¹⁷O of O₂ Data from Beyond EPICA Ice Core across the Mid-Pleistocene Transition (1.2 to 0.7 million years)  

Léa Baubant, Amaëlle Landais, Louisa Brückner, Anna Klüssendorf, Elodie Brugere, Frédéric Prié, Florian Krauss, Jochen Schmitt, Hubertus Fischer, and Stéphanie Duchamp-Alphonse and the Beyond EPICA Community

Within the framework of the Beyond EPICA project, the oldest continuous Antarctic ice core recovered to date provides, for the first time, direct measurements of the atmospheric composition over (at least) the past 1.2 million years (hereafter Ma), through the analysis of the air bubbles trapped in the ice. This interval encompasses the Mid-Pleistocene Transition, marked by a shift in the dominant climatic periodicity from ~40 ka to ~100 . Interestingly, preliminary results show that this time interval also witnesses a long-term decline in the atmospheric dioxygen (O2). Despite being a period of major reorganization of the Quaternary glacial–interglacial climate system, the processes that drove the MPT remain debated. Several hypotheses have been proposed, involving changes in ice-sheet dynamics, ocean circulation or the radiative forcing of atmospheric CO₂. Because atmospheric CO₂ and O₂ are tightly coupled through biogeochemical processes, investigating the evolution of atmospheric O₂ across the MPT may provide additional constraints on the mechanisms underlying this fundamental climatic shift. Here, we focus on the concentration of the triple isotopic composition of O2 (Δ¹⁷O(O₂)), a proxy for global biosphere productivity when interpreted together with CO2 concentration. We present the evolution of Δ¹⁷O(O₂) including the first continuous records from the deepest section of the Beyond EPICA ice core (from 2400 m to 2507 m). This record has been obtained as a by-product measurement when analysing the O2, N2 and Ar elemental and isotopic composition hence without O2 purification. Although characterized by relatively low analytical precision so far, the dataset offers comparatively high temporal resolution. The new Δ¹⁷O(O₂) record also confirms previously reported trends over the last 0.7–0.8 Ma, supporting its robustness for investigating both long-term changes and glacial-interglacial variability. We compare the long-term evolution of Δ¹⁷O (O₂) with the observed decrease in atmospheric O₂, and examine the amplitudes of glacial–interglacial variations in Δ¹⁷O (O₂) relative to those of CO₂ over the past 1.2 Ma. It appears that variations in the Δ¹⁷O (O₂)–CO₂ relationship during specific glacial – interglacial cycles could reflect changes in the biosphere productivity warranting further investigation.

How to cite: Baubant, L., Landais, A., Brückner, L., Klüssendorf, A., Brugere, E., Prié, F., Krauss, F., Schmitt, J., Fischer, H., and Duchamp-Alphonse, S. and the Beyond EPICA Community: First Δ¹⁷O of O₂ Data from Beyond EPICA Ice Core across the Mid-Pleistocene Transition (1.2 to 0.7 million years) , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5716, https://doi.org/10.5194/egusphere-egu26-5716, 2026.

EGU26-5800 | Posters on site | CL1.2.8

Firn densification in East Antarctica – a detailed model-data comparison at Dome C and Little Dome CFirn densification in East Antarctica – a detailed model-data comparison at Dome C and Little Dome C 

Amaelle Landais, Claire-Mathilde Stucki, Romilly Harris-Stuart, Johannes Freitag, Laurent Arnaud, Ghislain Picard, Roxanne Jacob, Louisa Brückner, Frederic Parrenin, Marie Bouchet, and Anaïs Orsi and the Beyond EPICA team

Deep ice cores from the East Antarctic plateau provide unique continuous records for paleoclimate. While some proxies are recorded in the ice phase, others are recorded in the gas phase. Air enclosure occurs at several dozens of meters below the snow surface which leads to gas being always younger than the surrounding ice. Presenting the records measured on the gas and ice phases on the same chronology relies on the determination of the lock-in depth (LID) where air is isolated from the atmosphere. Two different methods can be used to determine past LID in ice core. On the one hand, firn densification models have been developed over the past 45 years to model progressive evolution densification from surface snow to ice over the top 60 -120 m and empirical determinations permit to link firn density to the lock in process. On the other hand, measurements of d15N of N2 in trapped air in ice cores provide information on the past evolution of the LID through the gravitationnal fractionation which leads to a linear relationship between d15N of N2 and firn diffusive height, itself directly linked to LID in the absence of any surface convective zone.    

Here, we present independent estimate of the LID at two neighboring central sites in East Antarctica, Dome C (DC) and Little Dome C (LDC) where the EDC and BELDC deep ice cores have been drilled. We present results from different firn densification models and measurements of d15N of N2 both in the open porosity in the upper snow and in bubbles trapped in ice over the penultimate deglaciation and last interglacial period. For both studies, the measurementsshow a coherent 10% shallower LID at LDC than at DC which is relatively large given the similar climatic conditions on these neighboring sites. The firn densification models used in this study are not able to reproduce both the LID difference of about 10% between the two sites and the LID increase over the glacial -interglacial transitions. Missing processes in the firn densification model might be related with variations in the physical properties of the surface snow and surface snow metamorphism. To explore this hypothesis, our study hence also includes high resolution profile of density and specific surface area measurements at both sites.

How to cite: Landais, A., Stucki, C.-M., Harris-Stuart, R., Freitag, J., Arnaud, L., Picard, G., Jacob, R., Brückner, L., Parrenin, F., Bouchet, M., and Orsi, A. and the Beyond EPICA team: Firn densification in East Antarctica – a detailed model-data comparison at Dome C and Little Dome CFirn densification in East Antarctica – a detailed model-data comparison at Dome C and Little Dome C, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5800, https://doi.org/10.5194/egusphere-egu26-5800, 2026.

EGU26-6220 | Orals | CL1.2.8

Reconstructed CO2 variability over the entire Pleistocene inferred from sedimentary leaf wax carbon isotopes from the Bay of Bengal 

Masanobu Yamamoto, Tomohisa Irino, Renata Szarek, Osamu Seki, Ayako Abe-Ouchi, and Masakazu Yoshimori

Reconstructing past CO2 concentrations is essential to understanding paleoclimates. However, the CO2 record beyond the 805-ky ice core is insufficient to understand the relationship between CO2 and climate. Results from new ice cores and blue ice samples are highly anticipated. Here, we present the proxy CO2 record from the last 2.6 million years including the Mid-Pleistocene Transition, as determined by the δ13C values of sedimentary leaf waxes at IODP Site U1445, which reflect changes in the C3/C4 vegetation ratio in East Peninsular India. Our results show that interglacial CO2 levels in the early Pleistocene were lower than preindustrial levels. Higher CO2 levels occurred during super-interglacial periods. CO2 covaries with benthic δ18O on the orbital timescale. A strong coupling continued throughout the Pleistocene. Interglacial CO2 variation shows longer cycles averaging ~300 kyr, with several glacial cycles bunched together. A cycle begins with benthic δ18O and δ13C maxima in a glacial period, followed by an abrupt increase and subsequent decrease in interglacial CO2 levels. This suggests that the collapse of large ice sheets triggered the release of accumulated ocean carbon into the atmosphere. The size of the glacial ice sheets and the accumulation of oceanic carbon controlled the extent of deglacial CO2 release.

How to cite: Yamamoto, M., Irino, T., Szarek, R., Seki, O., Abe-Ouchi, A., and Yoshimori, M.: Reconstructed CO2 variability over the entire Pleistocene inferred from sedimentary leaf wax carbon isotopes from the Bay of Bengal, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6220, https://doi.org/10.5194/egusphere-egu26-6220, 2026.

EGU26-6467 | Posters on site | CL1.2.8

The first millennial-resolution triple greenhouse gas record over the MPT using novel sublimation extraction/laser spectrometry 

Hubertus Fischer, Florian Krauss, Jochen Schmitt, Robin Heiserer, Lucas Silva, Thomas Stocker, Emilie Capron, Michaela Mühl, Xavier Fain, Roberto Grilli, Thomas Bauska, Lison Soussaintjean, Rachael Rhodes, Thomas Blunier, and the entire Beyond EPICA community

The Mid-Pleistocene Transition (MPT) is characterized by a shift from 40 kyr to 100 kyr glacial cycles and increasing glacial ice volume. The reason for this change is still a matter of debate, but a plausible explanation could be a long-term decline of greenhouse gas (GHG) radiative forcing during glacial times across the MPT, which would have allowed global ice sheets to grow over a longer time interval and to greater size.

Although recent developments in marine CO2 proxies (for example Nuber et al., 2025) and CO2 measurements on blue ice samples (Marks Peterson et al., 2025) have led to first results to constrain the atmospheric CO2 over the MPT, an ultimate answer to the question how glacial/interglacial radiative forcing changed over the MPT is still missing. Marine CO2 proxies are limited in terms of precision and accuracy, making it difficult to reconstruct CO2 changes smaller than app. 20 ppm. Blue ice records show stable mean CO2 (and CH4) over the MPT with surprisingly little glacial/interglacial variations. The latter is likely due to glaciological reasons specific for blue that do not impact the continuous Beyond EPICA deep ice core.

Using the novel Laser Sublimation Extraction and multi-beam Quantum Cascade Laser Absorption Spectrometer developed at the University of Bern (in particular for the Beyond EPICA ice core, where availability of ice as old as the MPT is extremely limited due to the glacial thinning) we are able to measure CO2 (and its carbon isotopic composition!), CH4, and N2O concentrations all on the same  ice core sample of only 15 g with highest precision and accuracy. We applied this technique to discrete samples from the Beyond EPICA ice core to reconstruct the first multi-millennial record for all three GHG over the MPT, which allows us to quantify changes in the total GHG radiative forcing. The preliminary results confirm minimal secular changes across the MPT, but in contrast to the blue ice record reveals significant glacial/interglacial variations in all three GHG.

This poster will introduce the analytical details of this unique analytical system, present the latest results for the Beyond EPICA greenhouse gas records and discuss the implications and limitations of these results for the interpretation of the MPT. 

References

Marks Peterson, J. et al., Ice cores from the Allan Hills, Antarctica, show relatively stable atmospheric CO2 and CH4 levels over the last 3 million years, Research Square preprint under review, https://doi.org/10.21203/rs.3.rs-5610566/v1.

Nuber, S. et al., Mid Pleistocene Transition caused by decline in atmospheric CO2, Research Square Preprint under review, DOI: https://doi.org/10.21203/rs.3.rs-6480074/v1.

How to cite: Fischer, H., Krauss, F., Schmitt, J., Heiserer, R., Silva, L., Stocker, T., Capron, E., Mühl, M., Fain, X., Grilli, R., Bauska, T., Soussaintjean, L., Rhodes, R., Blunier, T., and Beyond EPICA community, T. E.: The first millennial-resolution triple greenhouse gas record over the MPT using novel sublimation extraction/laser spectrometry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6467, https://doi.org/10.5194/egusphere-egu26-6467, 2026.

EGU26-7071 | ECS | Orals | CL1.2.8

Post-depositional geochemical processes in EPICA Dome C ice: implications for BE-OIC dust analysis 

Geunwoo Lee, Tobias Erhardt, Piers Larkman, Chantal Zeppenfeld, Sarah Jackson, Barbara Delmonte, Giovanni Baccolo, Pascal Bohleber, and Hubertus Fischer

The Beyond EPICA–Oldest Ice Core (BE-OIC) project successfully recovered the oldest continuous Antarctic ice core, extending back to at least 1.2 million years. This landmark achievement provides an unprecedented opportunity to address long-standing questions regarding the mechanisms underlying the Mid-Pleistocene Transition (MPT) (Barbante & Beyond EPICA Team, 2025). Among others, this core could be used to study past changes in atmospheric aerosol composition and here, in particular the geochemical composition of mineral dust.

However, deep ice is increasingly recognized as a “geochemical reactor”, in which primary mineral impurities undergo post-depositional transformations into secondary phases such as jarosite (Baccolo et al., 2021; Lanci et al., 2025). These alterations pose a major challenge for extracting reliable paleoclimate signals from the analysis of mineral dust trapped into old ice. As such, to avoid misinterpretation of dust-related proxy records, we need to better constrain the nature and extent of deep-ice geochemical processes.

Here, we investigate post-depositional geochemical alterations in the EPICA Dome C (EDC) ice core through elemental analysis of ten sections (55 or 110 cm long) spanning the depth of 282 to 3137 m. For the first time, we apply single-particle inductively coupled plasma time-of-flight mass spectrometry (sp-ICP-TOFMS) coupled to the Bern continuous flow analysis (CFA) system to EDC ice core analysis. This approach allows the separate quantification of dissolved and particulate elemental fractions and enables the characterization of the chemical composition of individual particles. Our results reveal extensive dissolution of primary minerals (e.g. hornblende-like phases), accompanied by the precipitation of secondary insoluble and soluble sulfates (e.g. jarosite, alunite), and possibly other Fe-oxide phases. These transformations are likely driven by localized acidic and oxidative microenvironments that develop during the metamorphism of deep ice, depending, to first order, on the growth of ice grains.

Our findings provide new insights into post-depositional geochemical processes in deep Antarctic ice and are crucial for ensuring robust paleoclimate reconstructions from dust records in the oldest ice cores, including BE-OIC. Notably, significant geochemical alteration is observed in EDC sections at temperatures of approximately −15 °C and above, indicating that, at the conditions encountered at EDC, these changes emerge at around −15 °C and intensify under warmer conditions. Given that BE-OIC ice of comparable age to EDC is colder while exhibiting similar dust concentration, the BE-OIC ice core may preserve a less geochemically altered, and therefore higher-quality, dust archive for periods already covered by the EDC record (<800 ka). On the other hand, portions of the BE-OIC stratigraphy extend to substantially greater ages, implying longer residence times in ice and a higher potential for post-depositional alterations.

How to cite: Lee, G., Erhardt, T., Larkman, P., Zeppenfeld, C., Jackson, S., Delmonte, B., Baccolo, G., Bohleber, P., and Fischer, H.: Post-depositional geochemical processes in EPICA Dome C ice: implications for BE-OIC dust analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7071, https://doi.org/10.5194/egusphere-egu26-7071, 2026.

EGU26-7227 | ECS | Posters on site | CL1.2.8

Quasi-non-destructive water isotope measurements in ice cores using femtosecond laser ablation 

Ioanna Bertsia Kanatouri, Robin Vinther Nielsen, and Vasileios Gkinis

We present a quasi-non-destructive technique for measuring water isotopes in ice cores using a femtosecond infrared laser ablation system. Our cold-ablation approach enables a direct solid-to-vapour transition with sub-millimetre resolution and negligible sample consumption. Experiments conducted on synthetic ice demonstrate reproducible crater formation. Utilising a pulse energy of 35 μJ and a total ablation time of 16 s, repeatable craters with a typical diameter of ∼120 μm are produced. The ablation is performed at atmospheric pressure and requires only compressed dry air.

We demonstrate a sequence of 530 craters along a 27 cm long standard CFA ice section (30 × 30 mm), with the capability to extend to a full 55 cm ice-core bag and to accommodate a complete 4″ round core. The crater spacing is 0.5 mm and a full ablation run takes approximately 30 min and is largely unattended. Finally, we present preliminary results on coupling a cavity ring-down spectroscopy (CRDS) instrument to the ablation system.

This development is relevant for very old and deep ice core samples, such as those targeted by the BEOIC project and other >1 Myr ice cores, where sample preservation and spatial resolution are crucial.

How to cite: Bertsia Kanatouri, I., Nielsen, R. V., and Gkinis, V.: Quasi-non-destructive water isotope measurements in ice cores using femtosecond laser ablation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7227, https://doi.org/10.5194/egusphere-egu26-7227, 2026.

EGU26-7309 | ECS | Orals | CL1.2.8

Orbital Dating of the Beyond EPICA Ice Core and Identification of Possible Stratigraphic Disturbances 

Louisa Brückner, Anna Klüssendorf, Léa Baubant, Elodie Brugère, Frédéric Prié, Frédéric Parrenin, Emilie Capron, Bénédicte Minster, Elise Fourré, Thomas Combacal, Sébastien Nomade, Franck Bassinot, and Amaëlle Landais and the Beyond EPICA water isotope team

The new Beyond EPICA Antarctic ice core plays a crucial role in deciphering the contribution and behaviour of atmospheric proxies before and during the Mid-Pleistocene transition. In order to fully understand and correctly interpret the connection between different proxies both from the ice and gas phase of the ice core, as well as from other climactic archives, an accurate chronology of the entire ice core is needed. This can be achieved with orbital dating, exploiting the unique relationship between insolation and some of the isotopic and elemental ratios of atmospheric constituents such as nitrogen, oxygen, and argon of the air bubbles trapped in the ice. Using new atmospheric δ18O of O2, δ(O2/N2), and δ(Ar/N2) data in the depth range between 2400-2507 m from the Beyond EPICA ice core, we propose new chronological tie points, which are independent of alignment to marine archives, for the construction of a gas and ice chronology of the Beyond EPICA ice core before 800,000 years before present.

Additionally, δ15N of N2 measurements provide a way to quantify variations in the lock-in depth and the age difference between the ice and the gas phase (Δage) over the entire time period covered by the Beyond EPICA ice core. The new δ15N dataset provided here is key for the coherence between the ice and gas timescale. Moreover, we use the expected depth difference (Δdepth) between the same event recorded in the ice phase (through δD or δ18O of the ice) and in the gas phase (through δ15N of N2) as a test for the integrity of the stratigraphy: a concomitant change in δD or δ18O of the ice and δ15N of N2 may be the signature of an ice hiatus or folding event.

How to cite: Brückner, L., Klüssendorf, A., Baubant, L., Brugère, E., Prié, F., Parrenin, F., Capron, E., Minster, B., Fourré, E., Combacal, T., Nomade, S., Bassinot, F., and Landais, A. and the Beyond EPICA water isotope team: Orbital Dating of the Beyond EPICA Ice Core and Identification of Possible Stratigraphic Disturbances, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7309, https://doi.org/10.5194/egusphere-egu26-7309, 2026.

EGU26-7431 | Orals | CL1.2.8

SW Iberian Margin 1500 ka (SWIM1500): A benchmark record for comparison with the Beyond EPICA-Oldest Ice (BE-OI) Core  

David Hodell, Rachael Rhodes, Eric Wolff, and Francesco Muschitiello

As nearly all the mass, heat capacity, and carbon in the ocean-atmosphere system resides in the deep sea, ice cores must be correlated and integrated with marine sediment cores to provide a comprehensive, dynamic understanding of Earth's past climate. The SW Iberian Margin (SWIM) is a well-known location where sediments accumulate at high rates and can be correlated precisely to the polar ice cores. With new drilling during IODP Expedition 397, we filled a 30-kyr hiatus in the previous record of Site U1385 across the MIS 12/11 transition (Termination V) and extended the record to MIS 53, which we call SWIM1500. For the last 800 kyrs, we demonstrate that CH4 and δD in the EPICA ice core can be precisely correlated on millennial time scales to the planktic and benthic δ18O proxies, respectively, using a new Bayesian algorithm for automated synchronization of proxy timeseries (e.g. Muschitiello and Aquino-Lopez, 2024) that factors in prior knowledge on accumulation rates.

We suggest that SWIM1500 can serve as a predictive tool for isotopic and CH4 variations for the new BE-OI core beyond 800 ka and will aid in evaluating disturbance and/or diffusion in the oldest ice. We focus on the period older than 1.2 Ma because the stratigraphy and chronology of the BE-OI core is less certain in this interval. The unique shapes of the glacial-interglacial cycles (related to the phasing of obliquity and precession) and nested glacial millennial variability offer a template for correlating and interpreting the BE-OI and Site U1385 records. These correlations will be particularly important for evaluating the climate background state in the "41-kyr world" before the beginning of the Middle Pleistocene Transition at 1.2 Ma.

Muschitiello, F. and Aquino-Lopez, M. A.: Continuous synchronization of the Greenland ice-core and U–Th timescales using probabilistic inversion, Clim. Past, 20, 1415–1435, https://doi.org/10.5194/cp-20-1415-2024, 2024. 

How to cite: Hodell, D., Rhodes, R., Wolff, E., and Muschitiello, F.: SW Iberian Margin 1500 ka (SWIM1500): A benchmark record for comparison with the Beyond EPICA-Oldest Ice (BE-OI) Core , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7431, https://doi.org/10.5194/egusphere-egu26-7431, 2026.

EGU26-7849 | ECS | Posters on site | CL1.2.8

 Exploring orbital-paced forcings impacts on the Mid-Pleistocene Transition using snapshot simulations 

Jeanne Millot-Weil, Paul Valdes, and Alexander Farnsworth
The change in ice age cyclicity from a 40-kyr to a 100-kyr pace between 750 kyr and 1,250 kyr called the Mid-Pleistocene Transition (MPT), has been widely observed from geological records.  While ice age cyclicity is commonly explained by insolation variations received at the top of the atmosphere, insolation forcing alone cannot explain the shift observed during the MPT, suggesting major impact played by the internal forcings like ice sheet variations and greenhouse gases concentrations. Previous works have highlighted the role of both these forcings along with a likely change of global ocean circulation. However, identifying the individual impacts of each forcing and whether ocean changes are a consequence of a driver of the MPT remains elusive.
Here, we use a recently updated version of HadCM3B paleoclimate model with realistic boundary conditions to explore orbital-scale drivers on global ocean circulation variations through the MPT. To this end, we take advantage of four recently extended sets of 919 snapshot simulations that cover the last 3.6 million years at ~4,000-year increments. They differ by their orbital timescale forcings: i) with changing insolation only (Pre-industrial ice sheet and GHG kept constant throughout), ii) with changing insolation and greenhouse gas variations only (Pre-industrial ice sheet kept constant throughout), iii) with changing insolation and ice sheet only (Pre-industrial GHG kept constant throughout) and iv) combining variations of insolation, greenhouse gas and ice sheet in unison.
After evaluating model’s results against geological reconstructions (with (Clark et al,. 2024) stacks in particular), we show the decisive impact of CO2 variations on global trends and ice age cyclicity shift during the MPT.  Ice sheet variations are mainly important to explain high latitudes changes and ice ages amplitude, driving then changes of ocean circulation strength.

How to cite: Millot-Weil, J., Valdes, P., and Farnsworth, A.:  Exploring orbital-paced forcings impacts on the Mid-Pleistocene Transition using snapshot simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7849, https://doi.org/10.5194/egusphere-egu26-7849, 2026.

EGU26-8430 | Orals | CL1.2.8

Pleistocene to late Miocene ice core records of climate and atmospheric composition from Allan Hills, Antarctica 

Ed Brook and the NSF Center for Oldest Ice Exploration Ice Coring and Analysis Participants

Under the auspices of the NSF Center for Oldest Ice Exploration and previous projects, multiple seasons of shallow ice core drilling in the Allan Hills Blue Ice Area have yielded ice samples as old as 6.7 Ma, and numerous younger samples beyond the current 800 ka limit of the traditional ice core record. The complex stratigraphy of the existing cores does not allow continuous time series. Instead, “snapshots” have been created by dating over 300 individual samples (with more coming) using the deficit in 40Ar compared to modern air, and analyzing those samples for a range of environmental parameters. Parallel efforts are using continuous flow analysis, continuous electrical conductivity measurements, geophysical observations and surface transects to further understand the preservation and stratigraphy of environmental records in this unique region. This presentation will review recent results including evolving data sets from ice cores collected in the last two years. Primary observations include 1) long term Antarctic cooling of up to ~12 ˚C over the last 6 Ma based on the stable isotopic composition of the ice; 2) long-term mean ocean cooling over the last 3 Ma based on atmospheric noble gas ratios, with a prominent period of cooling coincident with the Plio-Pleistocene transition (~2.7 Ma) and steady temperatures across the mid-Pleistocene transition (1.2-0.8 Ma); 3) atmospheric CO2 concentrations of less than 300 ppm in pristine ice back to 2.7 Ma, corroborated by similar levels reconstructed from ice samples affected by respiration near the glacier bed based on corrections using carbon isotopes or independent constraints based on mass independent fractionation of isotopes in O2; 4) moderate atmospheric methane levels back to 3 Ma (generally less than 600 ppb) with evidence for biologically produced methane in samples near the glacier bed; 5) age reversals and inclined layering from 3 dimensional electrical and chemical measurements, and evidence for both pristine glacial ice and interactions with the glacier bed that alter the ice chemistry. These emerging new Antarctic ice core records are enhancing scientific understanding of Plio-Pleistocene climate and planetary evolution. Ongoing efforts in method development, ice coring, and geochemical analysis will continue to provide new insights from this enigmatic and challenging ice archive.

How to cite: Brook, E. and the NSF Center for Oldest Ice Exploration Ice Coring and Analysis Participants: Pleistocene to late Miocene ice core records of climate and atmospheric composition from Allan Hills, Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8430, https://doi.org/10.5194/egusphere-egu26-8430, 2026.

EGU26-8488 | Posters on site | CL1.2.8

The Million Year Ice Core Project at Dome C North 

Joel B. Pedro and the Million Year Ice Core Project Team

The Million Year Ice Core (MYIC) Project is an Australian Antarctic Program initiative to recover a continuous ice core spanning the mid-Pleistocene Transition (MPT; 700–1,250kyr). MYIC pilot drilling and borehole reaming for casing installation started in the 2024/25 austral summer at Dome C North (DCN, 75.04220S, 123.63120E, ice depth of 3064 m). DCN is 9 km NE of Concordia Station and 45 km NE of the European Beyond EPICA Oldest Ice site at Little Dome C (LDC). In the 2025/26 season, casing was installed and deep drilling commenced using a new AAD deep drill system. Completion of drilling to bedrock is scheduled for the 2028/29 season.

One-dimensional ice modelling, constrained by ice penetrating radar and isochrones traced back to the original EPICA Dome C ice core site, indicate an age above the basal ice at DCN potentially reaching 2 million years (Ma) and a resolution at 1.5 Ma of 10,000 years per metre or better (Chung et al., 2023).

Laboratory capabilities for MYIC are directed at measurements required to test hypotheses on the cause of the MPT. Ice core continuous flow analysis (CFA) for conductivity, particles and soluble ions are underway, with fraction-collected aliquots taken for measurement of cosmogenic 10Be. Gas and water isotope measurements on the returned ice are scheduled to start this year. The new gas laboratory developed for the project combines a small-sample sublimation extraction system coupled to a Quantum Cascade Laser spectrometer and dual inlet mass spectrometry for combined measurement of CO2, δ13C-CO2, CH4, and N2O, as well as the main air isotopes. There are opportunities for measurements of other parameters through national and international collaboration.

How to cite: Pedro, J. B. and the Million Year Ice Core Project Team: The Million Year Ice Core Project at Dome C North, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8488, https://doi.org/10.5194/egusphere-egu26-8488, 2026.

EGU26-9284 | ECS | Posters on site | CL1.2.8

Assessing the issue of the water isotope signal loss in the BEOIC ice core. A model and high-resolution data perspective. 

Caroline Juelsholt, Bo Møllesøe Vinther, Maria Hörhold, Melanie Behrens, Frank Wilhelms, Johannes Freitag, Ilka Weikusat, Daniela Jansen, Thomas Laepple, Bénédicte Minster, Amaelle Landais, Hans Christian Steen-Larsen, Natthaporn Phumchat, Barbara Stenni, Matteo Salvini, Carlo Barbante, Frederic Parrenin, Emma Samin, Federico Scoto, and Vasileios Gkinis

A new deep ice-core record from the East Antarctic Plateau reaching at least 1.2 million years is now available through the Beyond EPICA Oldest Ice Core project (BEOIC). This record spans the Mid-Pleistocene Transition (MPT), when glacial-cycle pacing shifted from ~40 kyr to ~100 kyr, and therefore offers key constraints when combined water-isotope and greenhouse-gas measurements are interpreted together.

Recovering an accurate water-isotope signal from the deepest and oldest ice is challenging because diffusion in solid ice attenuates high-frequency variability. High-precision, high-resolution measurements combined with physically based estimates of isotope diffusion can be used to quantify signal attenuation and assess the feasibility of signal deconvolution.

Here, we present a combined modelling and data study that quantifies diffusion-driven attenuation of the water isotope signal along the BEOIC using updated age–depth information and borehole temperature constraints. We apply the resulting transfer functions to high-resolution isotope sections from multiple depths to evaluate the recoverable bandwidth and to test spectral/Wiener restoration approaches, including the impact of measurement noise and sampling resolution on the reconstruction.

How to cite: Juelsholt, C., Vinther, B. M., Hörhold, M., Behrens, M., Wilhelms, F., Freitag, J., Weikusat, I., Jansen, D., Laepple, T., Minster, B., Landais, A., Steen-Larsen, H. C., Phumchat, N., Stenni, B., Salvini, M., Barbante, C., Parrenin, F., Samin, E., Scoto, F., and Gkinis, V.: Assessing the issue of the water isotope signal loss in the BEOIC ice core. A model and high-resolution data perspective., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9284, https://doi.org/10.5194/egusphere-egu26-9284, 2026.

EGU26-9326 | ECS | Orals | CL1.2.8

A continuous record of particulate mineral dust from the new Beyond EPICA Oldest Ice Core: paleoclimatic implications of variability in dust physical and optical properties 

Sarah Jackson, Hubertus Fischer, Geunwoo Lee, Sophie Spelsberg, Barbara Delmonte, Jack Humby, Dieter Tetzner, Elizabeth Thomas, and Eric Wolff

Particulate mineral dust is a critical part of the Earth’s climate system, modulating radiative balance and providing a crucial source of micronutrients to surface oceans. In ice cores, mineral dust also serves as a key proxy for past atmospheric dynamics - controlling dust mobilization and transport - as well as hydroclimate variability, which affects the atmospheric residence time of dust in addition to emission strength in the source regions. Previous studies, including those from the 800,000-year EPICA Dome C ice core, have demonstrated a close coupling between dust particle number concentrations in ice cores and glacial-interglacial climate variability, with consistently higher dust concentrations during cold glacial periods. The new Beyond EPICA-Oldest Ice Core (BE-OIC: 75º 18’ S, 122º 27’ W) extends the existing ice core particulate dust record back through the Mid-Pleistocene Transition (MPT), providing new constraints on this enigmatic period in Earth’s climate history.

We present the first continuous record of particulate mineral dust particle size and particle number distributions from the new BE-OIC, spanning from 700,000 years BP through the Mid-Pleistocene Transition. Physical characteristics of individual dust grains were measured online by the University of Bern during the Continuous Flow Analysis measurement campaign at the British Antarctic Survey using dual Classizer One Single Particle Extinction and Scattering instruments (EOS) and an Abakus laser particle sensor (Klotz GmbH), enabling characterization of particle concentration, dust size but also its refractive index over a wide range of diameters (0.2–10 µm). The latter is crucial as it allows us for the first time to resolve the submicrometer mode in the number size distribution.

Consistent with earlier work on the EDC ice core, the new BE-OIC record shows elevated dust concentrations during glacial periods both before, during and post MPT. However, the amplitude of glacial-interglacial variability is reduced relative to the past 800,000 years. In addition, modal particle diameters in the number size distribution are smaller during glacials compared to interglacials, indicating enhanced contributions from long-distance dust transport during the colder climate states. We investigate the processes that lead to dust size and number changes, including how reduced glacial intensity pre-MPT may have impacted dust source regions and the atmospheric lifetimes of dust particles. Together, these observations indicate changes in dust source-to-sink dynamics that have implications for biogeochemical cycles in the Southern Ocean and atmospheric dynamics during the MPT.  

How to cite: Jackson, S., Fischer, H., Lee, G., Spelsberg, S., Delmonte, B., Humby, J., Tetzner, D., Thomas, E., and Wolff, E.: A continuous record of particulate mineral dust from the new Beyond EPICA Oldest Ice Core: paleoclimatic implications of variability in dust physical and optical properties, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9326, https://doi.org/10.5194/egusphere-egu26-9326, 2026.

EGU26-10015 | Posters on site | CL1.2.8

Millennial-scale jumps in total air content at Dome C and new total air content measurements over the MPT on the Beyond EPICA ice core 

Barbara Seth, Jochen Schmitt, Markus Grimmer, Heloise Guilluy, Emilie Capron, Frederic Parrenin, Anna Maria Klussendorf, Louisa Bruckner, Amaelle Landais, and Hubertus Fischer

Measurements of the total air content (TAC) in ice cores have a long history and were motivated to reconstruct past changes in the altitude of the ice sheet at the drill site, as air pressure is the dominant control on TAC. To allow this, one must know the porosity at bubble closure (pore volume) and correct for temperature. Temporal changes in the porosity are difficult to constrain, limiting its use as an altitude proxy. Orbital changes in the local insolation were found to modulate the TAC signal, allowing this parameter to be used as an additional orbital dating tool without a precise process understanding of the driving mechanism. Recent measurement campaigns on the EPICA Dome C ice core covering the last 450 kyr have increased the temporal resolution and allow about 1 kyr resolution between MIS 9 and MIS 7 (around 350 to 210 kyr). Our high-resolution record corroborated the well-known orbital TAC variations; however, it also showed rapid upward jumps within 2 kyr that were not previously visible. These TAC jumps are especially pronounced in MIS 7 and 9, interglacials characterised by so-called late deglacial overshoots in CO2 and CH4, but are also visible in water isotopes and aerosol records. The characteristic sequence for these overshoot interglacials is as follows:

From a TAC maximum that is reached already before the start of the deglaciation, TAC is slowly dropping to reach a pronounced minimum right at the interglacial temperature maximum.  After this minimum, TAC values rapidly increase within 2 kyr, thus less than the age of the firn column. This suggests that the millennial-scale changes in temperature and accumulation at the start of the interglacial lead to a transient disequilibrium in firnification. I.e., during the early interglacial warming, the rise in snow accumulation, hence overburden pressure, on top of a firn column leads to a transient creep-related reduction of porosity, hence to the pronounced TAC minima. Similar millennial-scale TAC features were observed in Greenlandic ice cores (Eicher et al. 2016) during rapid DO events.

With the advent of the Beyond EPICA ice core, we can now examine the characteristics of older interglacials to answer the question which of the interglacials during the MPT exhibit these dynamic TAC features and which resemble interglacials that seem to lack them (e.g. MIS 11). First measurements on the BEOI during the MPT indicate an orbital TAC dynamic similar to those over the last 600 kyr, while pronounced TAC minima characteristic of overshoots have not yet been identified. Moreover, the TAC evolution of MIS 31 seems to resemble the overall characteristics of MIS 11, i.e., it lacks the overshoot characteristics.        

How to cite: Seth, B., Schmitt, J., Grimmer, M., Guilluy, H., Capron, E., Parrenin, F., Klussendorf, A. M., Bruckner, L., Landais, A., and Fischer, H.: Millennial-scale jumps in total air content at Dome C and new total air content measurements over the MPT on the Beyond EPICA ice core, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10015, https://doi.org/10.5194/egusphere-egu26-10015, 2026.

EGU26-11375 | ECS | Posters on site | CL1.2.8

Multi-GHG analysis with the BigCIM: a novel system for fast and discrete ice core reconstructions 

Lucas Silva, Robin Heiserer, Florian Krauss, Remo Walther, Samuel Marending, Christoph Reinhard, Jochen Schmitt, Hubertus Fischer, and Thomas Stocker

Deep Antarctic ice cores can contain thousands of years of past climate history stored in a meter of ice. This limited sample availability demands experimental setups to extract the maximum amount of information while using the minimum amount of sample. Here we present the BigCIM (Big Centrifugal Ice Microtome), a novel system for discrete ice core measurements of atmospheric CO2, d13C-CO2, CH4 and N2O. Combining the fast dry extraction principle from the Centrifugal Ice Microtome (CIM; Bereiter et al., 2013), and the analytical capabilities of the Quantum Cascade Laser-based Absorption Spectrometer (QCLAS; Bereiter et al., 2020), the BigCIM requires 16-g cuboid samples and throughputs 5 samples/day. Blank measurements using standard gas over gas-free ice achieve precisions (1s) of 0.3 ppm for CO2, 0.06 permil for d13C-CO2, 2 ppb for CH4 and 1 ppb for N2O, comparable to other dry-extraction methods (Mächler et al., 2023). Preliminary results from the EDC ice core shows general agreement with previously published data. The ability to measure multiple gas species simultaneously on small samples at a relatively quick pace makes the BigCIM a suitable instrument for measuring late Pleistocene greenhouse gas records on BE-OI ice core.

REFERENCES 

 Bereiter, B., Stocker, T. F., and Fischer, H., A centrifugal ice microtome for measurements of atmospheric CO2 on air trapped in polar ice cores. Atmos. Meas. Tech., 6, 251-262 (2013). 

BereiterB. et al., High precision laser spectrometer for multiple greenhouse gas analysis in 1 mL air from ice core samples. Atmos. Meas. Tech., 13, 6391–6406 (2020). 

Mächler, L. et al., Laser-induced sublimation extraction for centimeter-resolution multi-species greenhouse gas analysis on ice cores. Atmos. Meas. Tech., 16, 355–372 (2023). 

How to cite: Silva, L., Heiserer, R., Krauss, F., Walther, R., Marending, S., Reinhard, C., Schmitt, J., Fischer, H., and Stocker, T.: Multi-GHG analysis with the BigCIM: a novel system for fast and discrete ice core reconstructions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11375, https://doi.org/10.5194/egusphere-egu26-11375, 2026.

EGU26-12810 | ECS | Posters on site | CL1.2.8

High-resolution ẟ18O and ẟ2H profiles from 700 to 800 kyr BP in the Beyond EPICA ice core: insights from a comparison with EPICA Dome C 

Matteo Salvini, Barbara Stenni, Enrico Biscaro, Amaelle Landais, Mauro Masiol, Giuliano Dreossi, Federico Scoto, Daniele Zannoni, Carlo Barbante, Emma Samin, and Frédéric Parrenin and the Beyond EPICA isotope and processing team

The Beyond EPICA project (BE-OI) has extended the oldest continuous ice core climate record, capturing at least 1.2 million years. The 2,800-meter-long core was drilled at Little Dome C (LDC) in the East Antarctic Plateau, 35 km south-east of Dome C (DC). BE-OI seeks to disentangle the Mid-Pleistocene Transition (0.9-1.2 Myr BP), a crucial period of Earth’s climate history when the shorter 41 kyr glacial cycles shifted to a dominant 100 kyr regime.

Paleotemperature reconstructions obtained from ice cores mainly rely on water stable isotopes (ẟ18O and ẟ2H). Variations in isotope ratios reflect changes in local temperature with less negative values characterizing warmer periods and more negative values associated with colder conditions. Past interglacial periods characterized by higher temperatures, higher sea levels, and reduced ice sheets provide valuable insights for investigating how different orbital configurations affect the climate system without the influence of northern hemisphere glacial ice sheets.

Within this framework, a preliminary comparative analysis was carried out between EPICA Dome C (EDC) and Beyond EPICA isotope records, with a focus on the climate variability between 700 and 800 kyr BP. This period covers two interglacials corresponding to the bottom part (3082-3189 m) of the EDC ice core including MIS 19 which represents the period with the closest orbital configuration parameters to the Holocene. In this study, high-resolution measurements of ẟ2H and ẟ18O were performed by means of Cavity Ring-Down Spectroscopy. Sample analyses were conducted with a sampling resolution of 2.5 cm using internal standards intercalibrated within the laboratories of the Beyond EPICA water isotope consortium. This high-resolution record is in good agreement with the low-resolution isotopic measurements performed in the field.  The captured climate variability has been compared with the EPICA record to assess the onset of potential new climatic information captured by water stable isotopes. To account for the differences between the two coring locations, the stable isotope composition of surface snow collected along an initial traverse between DC and LDC during the 2023–2024 field season will be considered, together with snow trench samples from both sites.

How to cite: Salvini, M., Stenni, B., Biscaro, E., Landais, A., Masiol, M., Dreossi, G., Scoto, F., Zannoni, D., Barbante, C., Samin, E., and Parrenin, F. and the Beyond EPICA isotope and processing team: High-resolution ẟ18O and ẟ2H profiles from 700 to 800 kyr BP in the Beyond EPICA ice core: insights from a comparison with EPICA Dome C, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12810, https://doi.org/10.5194/egusphere-egu26-12810, 2026.

EGU26-12940 | Posters on site | CL1.2.8

Coordinating Analytical Strengths for LA-ICP-MS Analysis of the Beyond EPICA Core 

Pascal Bohleber, Tobias Erhardt, Carlo Barbante, Remi Dallmayr, Piers Larkman, Rachael Rhodes, Marco Roman, Twishashish Roy, Nicolas Stoll, and Wolfgang Müller

The "Beyond EPICA Oldest Ice Core" (BE-OIC) collaboration has successfully recovered the Antarctic ice core BELDC (Beyond EPICA Little Dome C) reaching back at least 1.2 million years (Stenni et al., 2025). This record is expected to provide a crucial missing link for understanding the cause of the Mid-Pleistocene Transition. However, the extreme thinning of the deepest ice layers compresses more than 20k years in one meter, and thus calls for analysis at high spatial resolution going hand-in-hand with a rigorous assessment of stratigraphic integrity. For aerosol-related chemical impurities, post-depositional processes, such as diffusion, grain growth displacement, and geochemical reactions, are known to pose significant challenges for record preservation in deep ice.

Laser Ablation Inductively Coupled Plasma Mass Spectrometry (LA-ICP-MS) offers decisive advantages in this context by analysing the surface of solid ice samples at the micrometer scale (in the order of 1−100 μm). To fully exploit its potential for the BE-OIC project and to coordinate the LA-ICP-MS analysis of the BELDC deep sections, a dedicated "Laser Ablation Focus Group" has been established with members of AWI Bremerhaven and the Universities of Frankfurt, Venice and Cambrige. Here we present the first results of an ongoing "round robin" experiment designed to integrate the strengths of our different analytical systems. This intercomparison study utilizes shallow BELDC sections, covering both glacial and interglacial ice, which are currently analysed by two newly established systems: a broadband 2D mapping setup (AWI Bremerhaven; Bohleber et al., 2025) recently upgraded with a 33 cm cryogenic chamber for high throughput, and a dual-wavelength (157 & 193 nm) system optimized for high ablation efficiency of ice including a custom-designed cryo-holder (Uni Frankfurt; Erhardt et al. 2025).

By extending this inter-laboratory comparison to further LA-ICP-MS facilities of the focus group, we aim to establish a standardized framework for the BELDC deep-ice analysis and possibly also other future ice core projects. At the same time, our results provide the first LA-ICP-MS datasets for the BELDC core and indicate how these high resolution impurity datasets can be integrated with other methods, such as Continuous Flow Analysis (CFA). Ultimately, this collaborative effort aims to maximize the scientific output of LA-ICP-MS for the BE-OIC project by contributing to the most robust interpretation of this unique paleoclimate archive.

 

References

Bohleber, P., Stoll, N., Larkman, P., Rhodes, R. H., & Clases, D. (2025). New evidence on the microstructural localization of sulfur and chlorine in polar ice cores with implications for impurity diffusion. The Cryosphere, 19(11), 5485-5498. https://doi.org/10.5194/tc-19-5485-2025

Erhardt, T., Norris, C. A., Rittberger, R., Shelley, M., Kutzschbach, M., Marko, L., ... & Müller, W. (2025). Rationale, design and initial performance of a dual-wavelength (157 & 193 nm) cryo-LA-ICP-MS/MS system. Journal of Analytical Atomic Spectrometry, 40(10), 2857-2869. https://doi.org/10.1039/D5JA00090D

Stenni, B., Wilhelms, F., Westhoff, J., Alemany, O., Hansen, S., Dahl-Jensen, D., ... & Zannoni, D. (2025). The Beyond EPICA–Oldest Ice Core Project. European Association of Geochemistry. Goldschmidt 2025 Abstract. https://doi.org/10.7185/gold2025.29931

How to cite: Bohleber, P., Erhardt, T., Barbante, C., Dallmayr, R., Larkman, P., Rhodes, R., Roman, M., Roy, T., Stoll, N., and Müller, W.: Coordinating Analytical Strengths for LA-ICP-MS Analysis of the Beyond EPICA Core, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12940, https://doi.org/10.5194/egusphere-egu26-12940, 2026.

Several international projects aim to retrieve million-year-old ice from Antarctica. Most focus on obtaining a continuous climate record. In the about-to-start 5-year project Million-year Ice from Antarctica (MIA), we will conduct an observation-based assessment of the potential of a preserved climate record older than 1.5 Myr in the European flagship ice core, BEOIMIA will explore the “stagnant” ice zone, a roughly 200 m thick area of presumed stagnant ice that has not yet been characterised. In addition to exploiting its full paleoclimatic potential, MIA will advance our understanding of the ice dynamics of “stagnant" ice. This is highly relevant for ice sheets and glaciers and, thus, their impact on future sea level rise via solid ice discharge into the oceans. To accomplish these ambitious goals, we will apply a holistic approach. We will simultaneously analyse microstructural (e.g., grain size and shape, crystal-preferred orientation) and geochemical properties (e.g., impurity localisation) of solid ice samples using multiple methods. We will combine these measurements with the full-Stokes numerical ice flow model Underworld2, applying derived anisotropy data. We will also compare these results with the deepest sections of BEOI’s counterpart, the Million Year Ice Core (MYIC) project by the Australian Antarctic Division. MYIC is assumed to contain (almost) no “stagnant” ice. To fully exploit our interdisciplinary approach, we will analyse 2 COLDEX blue ice cores from the Allan Hills region, where the so-far-oldest ice on Earth was found. This contribution will outline the next five years of the MIA project and its potential to enhance our understanding of the oldest parts of the Antarctic Ice Sheet.

How to cite: Stoll, N.: Million-year Ice from Antarctica and the “Stagnant” Ice Zone: From Microstructure to Geochemistry (MIA:Mic2Geo) – linking BEOI’s “stagnant” ice, COLDEX’s Allan Hills blue ice, and Million Year Ice Core ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13041, https://doi.org/10.5194/egusphere-egu26-13041, 2026.

EGU26-13085 | Orals | CL1.2.8

No abrupt changes in CF4 emissions by granite weathering and erosion over the Mid-Pleistocene Transition  

Jochen Schmitt, Barbara Seth, Markus Grimmer, Florian Krauss, John Higgins, Valens Hishamunda, Edward Brook, Christo Buizert, Jane Willenbring, Peter Köhler, and Hubertus Fischer

The climate evolution over the Pleistocene (last 2.6 Myr) is characterised by a sequence of cold glacials that are interrupted by warmer interglacial phases. These glacial-interglacial cycles are expressed in changes in global ice volume, ocean temperature, and other parameters that serve as proxies to infer land and ocean processes or to provide information about radiative forcing changes.

The Mid-Pleistocene Transition (MPT; 1.2-0.9 Myr) is characterised by the transition from 41 kyr cycles to about 100 kyr cycles and likely a trend toward colder glacial periods. The Mid Brunhes (MB) marks a climate transition at about 450 kyr after which the interglacial intensity (e.g. temperatures and greenhouse gas concentrations) increased. Consolidated explanations of the causes of both the MPT and the MB are lacking. Internal climate dynamics or feedback mechanisms are required since frequencies and the power of orbital parameters did not systematically change over the last 1.2 Myr.

For the MPT, two main classes of explanations have been put forward to account for the advent of the 100-kyr cycles. One argues that the ice sheets grew larger because the glacial climate became colder, driven by a long-term decline in glacial CO2 (GHG forcing). The other argues that NH ice sheets survived the next potential termination because land-surface properties (e.g. regolith, routing of ice sheets) made them less sensitive to meltdown.  

Here, we present a record of CF4 measured on ice core samples from the EPICA and Beyond EPICA ice cores, as well as some even older samples from the Alan Hills blue ice area that may shed additional light on the potential reasons for the MB and MPT. CF4 is a natural gas with a very long lifetime (on the order of 100 kyr) occurring predominantly in granitic rocks and other acidic plutonites and is released during chemical weathering and erosion of these rocks. Granites are globally distributed but have a bias towards high northern latitudes (Laurentide region, Scandinavia). Accordingly, some connection of CF4 release to ice sheet extent is to be expected. Over the Pleistocene, the surfaces of these high northern areas have been intensively eroded, and we would expect that a removal of this regolith layer would have left a sizable imprint in our CF4 record. However, our CF4 record shows a rather gradual decline from 2.6 Myr BP toward its local minimum reached shortly before the MB. In contrast, our CF4 record is consistent with the view that the CF4 release is most sensitive to chemical weathering and thus to temperature and the hydrologic regime. While we observe moderate changes in the average long-term CF4 emission flux (several glacial-interglacial cycles), the dominant variability is between glacials and interglacials, with the interglacials exhibiting about 40% higher emissions than colder times. The post-MB increase in CF4 is thus most easily understood through increased weathering during the warmer post-MB interglacials.

Our work provides new constraints on the regolith hypothesis for the MPT, and the first record of Pleistocene granite weathering/erosion trends.

 

How to cite: Schmitt, J., Seth, B., Grimmer, M., Krauss, F., Higgins, J., Hishamunda, V., Brook, E., Buizert, C., Willenbring, J., Köhler, P., and Fischer, H.: No abrupt changes in CF4 emissions by granite weathering and erosion over the Mid-Pleistocene Transition , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13085, https://doi.org/10.5194/egusphere-egu26-13085, 2026.

EGU26-13238 | ECS | Orals | CL1.2.8

The Oldest Antarctic 10Be Ice Core Record: New Insights Into Geomagnetic and Solar Variability Across the MPT 

Alexis Lamothe, Mélanie Baroni, Ellyn Auriol, Valéry Guillou, Team Aster, Edouard Bard, Ruben Rittberger, Florian Adolphi, Raimund Muscheler, and Beyond EPICA Community

The Beyond EPICA Oldest Ice (BE-OI) ice core provides a unique opportunity to investigate geomagnetic and solar variability across the Mid-Pleistocene Transition (MPT) using cosmogenic nuclides. We present a new high-resolution (15 cm) 10Be concentration profile measured continuously between 2412 and 2502 m depth, representing the oldest and longest cosmogenic nuclide records obtained from an ice core.

Preliminary results reveal an exceptionally well-preserved signal of the Brunhes-Matuyama reversal, the last reversal, that occurred approximately 780 k years ago. The 10Be BE-OI profile across the Brunhes-Matuyama reversal demonstrates a significantly improved signal-to-noise ratio compared with the EPICA Dome C (EDC) ice core which exhibited sporadic 10Be spikes disturbing the geomagnetic record.

The continuous 10Be record allows us to provide valuable dating horizons by identifying geomagnetic reversals and excursions and by direct comparison with authigenic marine 10Be records. Ongoing work focuses on exploiting this record to reconstruct variations in geomagnetic field intensity and to evaluate its consistency with existing marine relative paleointensity (RPI) and authigenic 10Be stacks.

In parallel, we investigate the potential contribution of solar modulation to the 10Be signal based on the differences between RPI and BE-OI 10Be records. We discuss the perspectives offered by the BE-OI record for disentangling, for the first time, geomagnetic and solar influences on cosmogenic nuclide production across the MPT. These results will provide valuable information on geomagnetic field intensity and solar modulation during a key transition in Earth's climate system.

How to cite: Lamothe, A., Baroni, M., Auriol, E., Guillou, V., Aster, T., Bard, E., Rittberger, R., Adolphi, F., Muscheler, R., and Community, B. E.: The Oldest Antarctic 10Be Ice Core Record: New Insights Into Geomagnetic and Solar Variability Across the MPT, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13238, https://doi.org/10.5194/egusphere-egu26-13238, 2026.

EGU26-13891 | ECS | Orals | CL1.2.8

The first coarse-resolution Beyond EPICA CO2 record covering the Mid-Pleistocene Transition: Insights from long-term carbon-cycle dynamics 

Florian Krauss, Jochen Schmitt, Thomas Bauska, Emilie Capron, Roberto Grilli, Robin Heiserer, Lucas Silva, Thomas Stocker, Hubertus Fischer, and the entire Beyond EPICA community

The Mid-Pleistocene Transition (MPT; 1.25 – 0.8 Myr) marks a transition from the “41-kyr world”, in which the Earth alternated between cold and warm periods about every 41,000 years, to the “100-kyr world” in which the Earth remained predominantly under glacial conditions but was punctuated every 80,000 to 120,000 years by interglacial periods. Variations in orbital forcing, the “pacemaker of the ice ages”, are stable across the MPT and thus cannot be invoked as a driver of this transition. Thus, most hypotheses call upon a forcing that drives a secular change, a feedback in the Earth system that changes/emerges, or a combination of the two.

One hypothesis for the MPT suggests that a long-term decline in (glacial) atmospheric CO2 levels led to a cooling, facilitating the formation of extensive ice sheets in North America and a sea-level drop of approximately 70 m (Bintanja & van de Wal, 2008). Accordingly, decreasing atmospheric CO2 concentration may have played a central role in driving this global cooling. Despite recent advances in marine and ice core CO₂ reconstructions (Nuber et al., 2025; Marks Peterson et al., 2025) the change of greenhouse gas forcing across the MPT remains uncertain for CO2.

In order to investigate the role of atmospheric CO2 across the MPT, greenhouse gases and the stable carbon isotopic composition of CO213C-CO2) were measured on discrete ice core samples from the Beyond EPICA ice core. For this purpose, a coupled Laser induced sublimation extraction – Quantum Cascade laser Absorption Spectrometer (LISE-QCLAS) was used, allowing the simultaneous and semi-continuous extraction and measurement of CO2, CH4 and N2O as well as δ13C-CO2 on air samples of only 1 – 2 mL, corresponding to 10 – 15 g of ice.

This talk will present the first ice core data capable of capturing glacial–interglacial variations in atmospheric CO₂ across the MPT. Additionally, we will present the first unconditionally pristine measurements of δ13C-CO2 during the 41-kyr world. These data will allow us to explore the underlying biogeochemical processes that may be responsible for the new modes of atmospheric CO2 variability we have observed.

How to cite: Krauss, F., Schmitt, J., Bauska, T., Capron, E., Grilli, R., Heiserer, R., Silva, L., Stocker, T., Fischer, H., and Beyond EPICA community, T. E.: The first coarse-resolution Beyond EPICA CO2 record covering the Mid-Pleistocene Transition: Insights from long-term carbon-cycle dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13891, https://doi.org/10.5194/egusphere-egu26-13891, 2026.

EGU26-13905 | Posters on site | CL1.2.8

Multi-gas component measurements of Beyond EPICA ice older than 700 kyr 

Thomas Blunier and the Beyond EPICA fastCFA Team

The Beyond EPICA project has extended our continuous ice core archive to 1.2—potentially 1.5—million years before present, covering the Mid-Pleistocene Transition (MPT). Ice older than that of the original EPICA core, spanning up to 800 kyr, is preserved in approximately only 100 meters of core.

To analyse this invaluable ice, European laboratories will converge in Copenhagen in February–March 2026 with their equipment to conduct simultaneous measurements of as many gas components as possible. Planned analyses include CH₄, CO, N₂O, and isotopes of O₂, N₂, and Ar. Since a methane record is a specific deliverable of the Beyond EPICA project, the campaign is designed to achieve the highest-resolution methane data possible.

The method involves melting a 3.5 × 3.5 cm ice stick on a specialised melt head. The inner, clean portion of the meltwater is then directed through a membrane system that separates the ancient air from the water. The meltwater itself is analysed for conductivity and dust content to synchronise the gas record with detailed chemical measurements of the core. The liberated air is analysed in real time using a suite of instruments. For the full set of gases, we combine two mass spectrometers with three laser spectrometers.

We will report on the outcome of the measurement campaign and present the first results.

How to cite: Blunier, T. and the Beyond EPICA fastCFA Team: Multi-gas component measurements of Beyond EPICA ice older than 700 kyr, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13905, https://doi.org/10.5194/egusphere-egu26-13905, 2026.

EGU26-14053 | Orals | CL1.2.8

Changes in Deep Circulation and Carbon Storage in the Eastern North Atlantic Ocean Across the Mid-Pleistocene Transition 

Jerry McManus, Celeste Pallone, Apollonia Arellano, Macy Mathews, Tim Kenna, Montserrat Alonso-García, Elizabeth Roxana Lasluisa Molina, Yaiza Kinney, Erin Kim, Brooke Harrison, Isabel Plower, Abigail Sturley, and Alexia Pryor

The duration and magnitude of Earth’s glaciation cycles increased substantially during the course of the Pleistocene without an obvious shift in external forcing. Changes in ocean circulation have been posited as one potential influence on this mid-Pleistocene transition (MPT). New drilling of a depth transect of sites on the Iberian margin during IODP Expedition 397 offers the opportunity to examine the record of deep-ocean circulation changes in the eastern north Atlantic over a range of bottom depths and water masses. Benthic carbon isotopes (d13C) and sedimentary characteristics that reflect bottom water conditions at Site U1587 (37°35′N, 10°22′W, 3.5 km) reveal persistent glacial-interglacial changes throughout the Pleistocene, with a shift toward larger and longer glacial cycles evident in benthic oxygen isotopes (d18O) across the MPT. A comparison with shallower Site U1385 (37°34′N 10°08′W 2.6 km) indicates that the vertical carbon-isotope gradient over this water depth also increased across the transition, particularly within glacial intervals, with far more negative d 13C at the deeper Site U1587. Uranium and thorium isotope analyses also indicate intervals of reduced dissolved oxygen and the deposition of authigenic uranium at greater depth. These observations suggest greater stratification and carbon storage in the deep eastern north Atlantic after the MPT, and support a likely role for ocean circulation in this important climate transition.

How to cite: McManus, J., Pallone, C., Arellano, A., Mathews, M., Kenna, T., Alonso-García, M., Lasluisa Molina, E. R., Kinney, Y., Kim, E., Harrison, B., Plower, I., Sturley, A., and Pryor, A.: Changes in Deep Circulation and Carbon Storage in the Eastern North Atlantic Ocean Across the Mid-Pleistocene Transition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14053, https://doi.org/10.5194/egusphere-egu26-14053, 2026.

EGU26-14467 | Posters on site | CL1.2.8

Ultra-High-resolution ẟ18O and ẟ2H measurements on the Beyond EPICA ice core: new insights into signal preservation 

Hans Christian Steen-Larsen, Natthaporn Phumchat, Vasileos Gkinis, Barbara Stenni, Giuliano Dreossi, Daniele Zannoni, Maria Hörhold, Melanie Behrens, Frank Wilhelms, Johannes Freitag, Ilka Weikusat, Daniela Jansen, Thomas Laepple, Bénédicte Minster, Amaëlle Landais, and Elisabeth Isaksson

While most of the below 700ka section of the Beyond EPICA ice core has been measured for water isotopic composition in 2.5 cm samples, a sub-section (depth 2473-2475 meters) has been cut into 1.25 cm. These ultra-high-resolution samples have been measured side-by-side with the 2.5 cm samples from the same depth, allowing a direct comparison with minimal calibration or instrument drift-induced uncertainty.  With great care for optimal measurement quality, we present here a comparison of the samples, with average precisions (+/- 1 STD) of 0.03 o/oo and 0.07 o/oo for ẟ18O and ẟ2H, respectively, and average accuracies of 0.03 o/oo and 0.4 o/oo for ẟ18O and ẟ2H, respectively.

Variations between the 1.25 cm and 2.5 cm samples that cannot be attributed to measurement uncertainty are observed. Our ultra-high-resolution measurements provide critical insights into intra-core variability, and we argue that ice cores, when possible, should be measured at the highest resolution to obtain optimal information about past climate variability.

How to cite: Steen-Larsen, H. C., Phumchat, N., Gkinis, V., Stenni, B., Dreossi, G., Zannoni, D., Hörhold, M., Behrens, M., Wilhelms, F., Freitag, J., Weikusat, I., Jansen, D., Laepple, T., Minster, B., Landais, A., and Isaksson, E.: Ultra-High-resolution ẟ18O and ẟ2H measurements on the Beyond EPICA ice core: new insights into signal preservation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14467, https://doi.org/10.5194/egusphere-egu26-14467, 2026.

EGU26-15092 | ECS | Posters on site | CL1.2.8

Characterisation and Correlation of Visible Tephra Horizons in the Beyond EPICA Oldest Ice Core 

Carys Thomas, Siwan Davies, Barbara Delmonte, Marco Rabassi, Paul Albert, William Hutchison, Sergio Andò, and Emma Watts

Antarctic ice cores provide exceptional archives of past climates and volcanic activity. Advances in sampling and analytical techniques are now enabling the detection and characterisation of both visible and cryptotephra deposits across increasingly long climate records. The Beyond EPICA Oldest Ice (BE-OI) project recently recovered what is thought to be the longest continuous Antarctic ice core. This core likely reaches back to ca. 1.2 million years, offering a unique opportunity to refine the chronology of glacial–interglacial cycles and the Mid-Pleistocene Transition. Here we present six visible tephra horizons identified within the upper 1850 m of the BE-OI record, thought to be originating from volcanic sources across the Antarctic region and beyond. These tephra deposits have modelled ages of 10.3, 70.3, 89.8, 142, 189 and 200 ka. Within this study, we explore potential correlations to tephras in the EPICA Dome C record.

Grain-size measurements, obtained through Coulter Counter analysis, together with optical microscopy and high-resolution single grain mineralogical data, have established the physical characteristics of the six tephra layers. Major element compositions determined by electron microprobe analysis and trace element data generated by LA-ICP-MS provide geochemical fingerprints for each deposit and point towards volcanic sources such as the South Sandwich Islands and Marie Byrd Land. The combination of these datasets enables robust tephra characterisation and supports correlations with established Antarctic tephra horizons. This work directly contributes to the refinement of the Beyond EPICA Oldest Ice chronology and its integration with the EPICA Dome C record.

How to cite: Thomas, C., Davies, S., Delmonte, B., Rabassi, M., Albert, P., Hutchison, W., Andò, S., and Watts, E.: Characterisation and Correlation of Visible Tephra Horizons in the Beyond EPICA Oldest Ice Core, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15092, https://doi.org/10.5194/egusphere-egu26-15092, 2026.

EGU26-15296 | Orals | CL1.2.8

New insights from the basal section of the Beyond EPICA ice core (Little Dome C)  

Pierre-Henri Blard, Julien Westhoff, Louise Crinella, François Fripiat, Frank Wilhelms, and Lisa Ardoin and the Beyond EPICA community

The basal section of the 2,800-m-long Beyond EPICA ice core (the lowermost 316 m) is of particular interest, not only because it potentially represents the oldest part of the core, but also because it contains important clues about past and present ice-sheet dynamics. We present here field observations and ongoing analyses aimed at characterizing the different ice units above the basal interface. Below the bottom of the “stratified ice” at 2,506 m, electrical conductivity, water-isotope composition, and crystal size allow the identification of a thinned and distorted zone extending down to 2,583 m, with no clear evidence of preserved climatic cycles. Below 2,583 m, the conductivity signal shows a sharp increase that persists over more than 200 m, although with some variability, and is associated with a marked increase in ice crystal size, reaching more than 10 cm.

The first occurrence of basal rock debris is observed at 2,795 m, where sand-sized and finer particles are embedded within the ice matrix, together with a few angular centimettric pebbles. This debris-rich section exhibits a heterogeneous composition, with decameter-scale alternations of banded, dispersed facies and clear-ice intervals. Density estimates of these basal units indicate that debris generally accounts for less than 1% of the mass, although it may locally reach a few percent. Two angular pebbles with volumes of several cubic centimeters are currently being processed for luminescence dating. Mineralogical observations suggest multiple source lithologies, supporting the hypothesis that the debris result from lateral transport and that the core did not reach the underlying bedrock. Scanning electron microscopy (SEM) observations of grain textures, together with geochemical analyses (Sr and Nd isotopes) and gas content will add additional constraints and help refine this interpretation and look for possible evidences of past deglaciation events. In addition, clay minerals and large (by XRD) will be analyzed to identify partially melted basal conditions in the past or weathering during ice free conditions.

 

How to cite: Blard, P.-H., Westhoff, J., Crinella, L., Fripiat, F., Wilhelms, F., and Ardoin, L. and the Beyond EPICA community: New insights from the basal section of the Beyond EPICA ice core (Little Dome C) , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15296, https://doi.org/10.5194/egusphere-egu26-15296, 2026.

EGU26-18402 | Orals | CL1.2.8

A challenge for Beyond EPICA Oldest Ice: Predictions of greenhouse gases across the MPT 

Thomas Bauska, Florian Krauss, Michaela Mühl, Lison Soussaintjean, Lucas Silva, Robin Heiserer, Hubertus Fischer, Jochen Schmitt, Thomas Stocker, Emilie Capron, Xavier Fain, Roberto Grilli, Rachael Rhodes, and Thomas Blunier

Understanding the drivers of the Mid-Pleistocene Transition (MPT) remains one of the most challenging problems in palaeoclimate. One unfulfilled prerequisite for tackling this problem is a comprehensive view of greenhouses gases (GHGs) across the MPT. The Beyond EPICA Oldest Ice project and other ice core efforts are now focused on extending the ice core record of GHGs through the MPT. As the new data emerges, it is useful to define a set of testable hypotheses - in this case, using predictions of GHGs across the MPT.

Most work on extending GHGs beyond the current ice core record have focused solely on predicting atmospheric CO2, although it is recognized that the combined radiative impact of CH4 and N2O could be of overlooked importance. The methods vary in complexity from statistical approaches using ocean sediment data - to box modelling efforts with prescribed forcings - to inversion methods targeting proxy data with a hierarchy of models - to earth system modelling with minimal (but none-the-less important) assumptions about external forcings.

Here we will build up an objective overview of these predictions. First, we review previous work from the literature. Second, we explore some new statistical models for all three GHGs, with a particular focus on utilizing high-resolution sediment records that capture millennial- and orbital-scale variability (Hodell et al., 2023) as well as highlighting the implications of new estimates of global surface temperature and ice volume (Clark et al., 2024). Finally, we provide novel histories using a combination of box model and published climate model data (Yun et al., 2023) that also go beyond predicting just CO2 and allow us to discuss coeval changes in CH4, N2O and δ13C-CO2.

This synthesis will provide one possible template for interpreting the new datasets that will be presented elsewhere. In particular, we will breakdown the various hypotheses in terms of changes in the mean and range of variability over the past 1.5 million years (i.e. the changes in overall mean, the glacial minima, and interglacial maxima). Furthermore, we will investigate how covariations of greenhouse gases concentration and isotopic composition can constrain the nature of biogeochemical feedbacks operating in the earth system across the MPT.

References

Clark, P.U, et al. (2025) Global mean sea level over the past 4.5 million years. Science 390, eadv8389, DOI:10.1126/science.adv8389

Hodell, D. A.,et al. (2023) A 1.5-million-year record of orbital and millennial climate variability in the North Atlantic, Clim. Past, 19, 607–636, https://doi.org/10.5194/cp-19-607-2023.

Yun, K.-S.,et al. (2023) A transient coupled general circulation model (CGCM) simulation of the past 3 million years, Clim. Past, 19, 1951–1974, https://doi.org/10.5194/cp-19-1951-2023

How to cite: Bauska, T., Krauss, F., Mühl, M., Soussaintjean, L., Silva, L., Heiserer, R., Fischer, H., Schmitt, J., Stocker, T., Capron, E., Fain, X., Grilli, R., Rhodes, R., and Blunier, T.: A challenge for Beyond EPICA Oldest Ice: Predictions of greenhouse gases across the MPT, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18402, https://doi.org/10.5194/egusphere-egu26-18402, 2026.

EGU26-18696 | Posters on site | CL1.2.8

Combined benthic clumped isotope and osmium isotope data over the Mid-Pleistocene transition: towards better constraints on the weathering and seawater temperatures and d18O 

Marion Peral, Inigo Müller, Lucien Nana Yobo, Thibaut Caley, Steven Goderis, and Philippe Claeys

The Mid-Pleistocene transition (MPT) is marked by a progressive increase of glacial-interglacial cycle amplitude, a shift of the climatic response from a 41-ka cycle dominated to a 100 ka-cycle, a prominent asymmetry in large glacial inceptions and an extension of glaciation. This transition is associated with a cooling of the sea surface temperatures and an increase of the atmospheric CO2 concertation, that could be associated with a change in the ice-sheet volume. One of the hypotheses to explain the MPT transition is the regolith hypothesis, based on the basal erosion of glaciers, resulting in changes in weathering and in ice-sheet volume. Here, we apply clumped isotope thermometer (Δ47) to benthic foraminifera. The Δ47 has also the advantage to be independent of the isotopic composition of the seawater (δ18Osw). As consequence, by combining Δ47 and δ18O from benthic foraminifera, the δ18Osw can be reconstructed. Our data are compared to osmium (Os) isotope measurements to observe potential change in weathering intensity. Thanks to this unique combination of Os isotope and Δ47, we can test the regolith hypothesis. We therefor present a new deep temperature dataset, combined with osmium, over the MPT, from the “Shackleton” site (IODP U1385 from exp. 397) in the North Atlantic Ocean.

The deep-temperatures show an unexpected increase between MIS 30 and MIS 22, associated to an increase of δ18Osw, while the osmium isotope decrease, indicated a decrease of weathering. These results point toward the regolith hypothesis with changes in ice sheet volume and weathering.

How to cite: Peral, M., Müller, I., Nana Yobo, L., Caley, T., Goderis, S., and Claeys, P.: Combined benthic clumped isotope and osmium isotope data over the Mid-Pleistocene transition: towards better constraints on the weathering and seawater temperatures and d18O, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18696, https://doi.org/10.5194/egusphere-egu26-18696, 2026.

EGU26-18791 | ECS | Posters on site | CL1.2.8

New Constrains on the History of the Greenland Ice Sheet from Krypton-81 Age Estimates 

Josephine Kande, Anders Svensson, Amaëlle Landais, Elise Fourré, Xin Feng, Wei Jiang, Qiao-Song Lin, Zheng-Tian Lu, Jie S. Wang, Guo-Min Yang, and Dorthe Dahl-Jensen

Understanding Greenland Ice Sheet (GrIS) variability over million-year timescales is critical for assessing its long-term stability and sensitivity to climate change. This study presents a synthesis of published evidence on past ice-free and ice-covered conditions in Greenland, integrating multiple paleoclimatic methods and datasets to provide a coherent overview of GrIS evolution. This outline highlights key intervals of changes in ice cover, such as warm and interglacial periods that are older than the last interglacial but remain less explored. Special attention is given to the Mid-Pleistocene Transition (MPT), when global glacial cycles shifted from 41 kyr to 100 kyr periodicity, potentially forming the basis for the present-day ice sheet geometry and state. Plausible scenarios for the GrIS respond to these periods will be explored and discussed based on the outline of evidence.

In addition to the synthesis, new age constraints from the Green2Ice project refine the existing picture. Novel krypton-81 dating of deep ice from the GRIP core reveals ice as old as 856 (+35/-33) ka, indicating persistent ice cover in central Greenland for nearly one million years. This finding provides a key point for evaluating model simulations and assessing physically meaningful scenarios for GrIS. Furthermore, these new results help test the hypotheses of significant ice sheet reorganization during the MPT.

By comparing evidence of ice-cover and ice-free conditions across methods and locations, this work explores areas of strong coherence and remaining uncertainties in Greenland’s long-term history. These insights not only improve our understanding of past GrIS behaviour but also inform projections of its future response under ongoing climate change.

How to cite: Kande, J., Svensson, A., Landais, A., Fourré, E., Feng, X., Jiang, W., Lin, Q.-S., Lu, Z.-T., Wang, J. S., Yang, G.-M., and Dahl-Jensen, D.: New Constrains on the History of the Greenland Ice Sheet from Krypton-81 Age Estimates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18791, https://doi.org/10.5194/egusphere-egu26-18791, 2026.

EGU26-19245 | ECS | Orals | CL1.2.8

Halogen Records from the Beyond EPICA Ice Core: Insights from the Holocene to the Mid-Pleistocene Transition 

Ginevra Chelli, Federica Bruschi, David Cappelletti, Mirko Severi, Rita Traversi, Elena Di Stefano, Azzurra Spagnesi, Valentina Raspagni, Barbara Stenni, Elena Barbaro, Marco Roman, Chiara Venier, Warren Cairns, Barbara Delmonte, Carlo Barbante, Chiara Petroselli, and Andrea Spolaor

Halogens (Br, I) and their enrichment relative to seawater abundance preserved in polar ice cores are powerful tracers for reconstructing past sea-ice dynamics and marine primary productivity. Within the framework of the Beyond EPICA Oldest Ice (BEOI) project, we present a new halogen concentration record derived from discrete ice core samples. Analytical measurements were performed in Italy (ISP-CNR, Ca’ Foscari University), focusing on the relatively stable climatic conditions of the Holocene and on the Mid-Pleistocene Transition (MPT).

The Holocene record, combined with previously published datasets, provides a critical baseline for understanding the environmental processes and transport mechanisms controlling halogen deposition on the central Antarctic plateau. To validate the halogen signal, we investigate the behaviour of bromine and iodine measured in the Younger Ice section of the BEOI ice core during the Holocene, comparing these records with independent paleoclimatic parameters from earlier studies, including temperature reconstructions (ΔT), stable water isotopes (δD), and sea surface temperatures (SST). These comparisons support the interpretation of halogen variability as a proxy for changes in sea-ice conditions.

While the Holocene analysis aims to constrain the halogen signal using well-established climatic parameters, the primary objective of the Beyond EPICA mission is to extend this approach back to 1.5 million years. As drilling reaches the deepest sections of the BEOI ice core, halogen records offer a unique opportunity to investigate changes in sea-ice dynamics across the MPT, when Earth’s climate system transitioned from a dominant 41-kyr to a 100-kyr glacial cyclicity. Ongoing chemical analyses of the oldest ice will help assess whether sea-ice feedbacks played a causal role in the emergence of the 100-kyr cycles or primarily acted as an amplifier of late-Pleistocene glacial intensification.

How to cite: Chelli, G., Bruschi, F., Cappelletti, D., Severi, M., Traversi, R., Di Stefano, E., Spagnesi, A., Raspagni, V., Stenni, B., Barbaro, E., Roman, M., Venier, C., Cairns, W., Delmonte, B., Barbante, C., Petroselli, C., and Spolaor, A.: Halogen Records from the Beyond EPICA Ice Core: Insights from the Holocene to the Mid-Pleistocene Transition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19245, https://doi.org/10.5194/egusphere-egu26-19245, 2026.

EGU26-20176 | Orals | CL1.2.8

Integrity and Interpretation of the Beyond-EPICA Oldest Ice core isotope record between 1 and 1.5 Mio years 

Thomas Laepple, Maria Hörhold, Daniela Jansen, Ilka Weikusat, Johannes Freitag, Frank Wilhelms, Melanie Behrens, Hanno Meyer, Hans Christian Steen-Larsen, Amaelle Landais, and Fyntan Shaw and the Beyond-EPICA isotope consortium

Which parts of the oldest ice-core water-isotope record can be trusted as a climate archive, and at what temporal resolution is the climatic information preserved?

The water-isotope record from the Beyond EPICA ice core represents the oldest continuous Antarctic ice-core climate archive, extending back to ~1.5 million years and uniquely covering the Mid-Pleistocene Transition. However, the deepest sections of ice cores are commonly affected by ice-flow-induced deformation that can distort the original stratigraphy. In addition, local depositional and post-depositional processes, as well as isotopic diffusion, progressively alter and smooth the climatic signal preserved in water isotopes.

Here, we assess the integrity and effective resolution of the Beyond EPICA water-isotope record by analysing its variability and comparing statistical properties of the measured signal with expectations derived from younger interglacials, other paleoclimate archives, and theoretical estimates of isotopic diffusion. This analysis is complemented by Dielectric Profiling (DEP) and optical line-scan data, which provide independent constraints on stratigraphic continuity and ice-core integrity. Together, these approaches allow us to begin assessing which parts of the Beyond EPICA record between 1.0 and 1.5 million years retain coherent climatic information, and to place first-order constraints on its temporal resolution.
 

How to cite: Laepple, T., Hörhold, M., Jansen, D., Weikusat, I., Freitag, J., Wilhelms, F., Behrens, M., Meyer, H., Steen-Larsen, H. C., Landais, A., and Shaw, F. and the Beyond-EPICA isotope consortium: Integrity and Interpretation of the Beyond-EPICA Oldest Ice core isotope record between 1 and 1.5 Mio years, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20176, https://doi.org/10.5194/egusphere-egu26-20176, 2026.

EGU26-20717 | Orals | CL1.2.8

Southern Ocean Marine Productivity across the Super-Interglacial MIS31 Reconstructed from Sulfur Isotopes from the Beyond EPICA Ice Core 

Andrea Burke, Yun-Ju Sun, Priyesh Prabhat, Rachael Rhodes, Margareta Hansson, Mengwen Yang, Patrick Sugden, Helen Innes, Helena Pryer, Joel Savarino, Hubertus Fischer, Eric Wolff, and Liz Thomas and the Beyond EPICA Oldest Ice Core Impurities CFA Team

Marine productivity in the Southern Ocean is thought to exert a key control on atmospheric CO2 concentrations in the past, present, and likely into the future. However, understanding how marine productivity responds to changes in ice sheet size and sea ice extent is challenging due to the limits of the observational record and the sensitivity of marine sediment core paleo-productivity records to the frontal shifts which accompany major climate changes. Sulfur isotopes in Antarctic ice cores provide a valuable new means of reconstructing past changes in Southern Ocean productivity as they enable the quantification of the contribution of different sulfate sources through isotope mass balance. Marine biological productivity is the major source of sulfate to the Antarctic ice sheet, and quantifying how that source has varied through time allows for a regionally integrated record of Southern Ocean primary productivity. Here we apply this method over the Super-Interglacial MIS31 and contrast it with more recent interglacials to investigate the response of Southern Ocean primary productivity to higher temperatures and a collapsed West Antarctic Ice Sheet.

How to cite: Burke, A., Sun, Y.-J., Prabhat, P., Rhodes, R., Hansson, M., Yang, M., Sugden, P., Innes, H., Pryer, H., Savarino, J., Fischer, H., Wolff, E., and Thomas, L. and the Beyond EPICA Oldest Ice Core Impurities CFA Team: Southern Ocean Marine Productivity across the Super-Interglacial MIS31 Reconstructed from Sulfur Isotopes from the Beyond EPICA Ice Core, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20717, https://doi.org/10.5194/egusphere-egu26-20717, 2026.

EGU26-20791 | Orals | CL1.2.8

Continuous CO2 reconstruction across the MPT from boron isotopes informs mechanisms of glacial CO2 change 

James Rae, Sophie Nuber, Thomas Chalk, Xuan Ji, Meike Scherrenberg, Timothy Heaton, Xu Zhang, Lennert Stap, Molly Trudgill, Heidi Block, Zhimin Jian, Chen Xu, Kaoru Kobata, Morten Andersen, Stephen Barker, Jimin Yu, and Gavin Foster

The Mid-Pleistocene Transition (MPT) represents a fundamental shift in the operation of Earth’s climate system, yet the role of CO2 in this transition is uncertain.  Prior to the MPT, the climate system was paced by the ~40 kyr obliquity cycle, with available CO2 reconstructions, temperatures, and ice volume all coupled to orbitally-forced changes in solar energy at high latitudes.  Following the MPT, this relationship breaks down, with Northern Hemisphere ice sheets persisting through obliquity maxima in a series of “skipped terminations”, leading to longer glacial periods with larger ice sheets.  Here we examine the role of CO2 over the MPT, using high resolution boron isotope data from 3 sediment cores, spanning the Atlantic, Pacific, and Indian Oceans.  These records show excellent agreement with the ice core record in their younger portions, and striking consistency between sites, supporting the robustness of our reconstruction of atmospheric CO2.  We find that CO2 and benthic oxygen isotopes remain largely coupled through the MPT, with limited CO2 rise during the skipped terminations around MIS 36 and 34, notably low CO2 during the deep glaciation of MIS 22 (the “900 ka event”), and notably high CO2 during the “super-interglacial” of MIS31.  This underscores the key role of CO2 in glacial and interglacial climate states.  In addition, it highlights that the mechanisms governing glacial-interglacial CO2 change, which are thought to be largely centred on the Southern Ocean, are not forced by orbital changes alone, but must be linked to land ice volume, as the only feature of the climate system with the inertia to persist through orbital insolation peaks.  This implies the existence of teleconnections between Northern Hemisphere ice volume and Southern Ocean CO2 storage, and we outline potential mechanisms by which this might be achieved. 

How to cite: Rae, J., Nuber, S., Chalk, T., Ji, X., Scherrenberg, M., Heaton, T., Zhang, X., Stap, L., Trudgill, M., Block, H., Jian, Z., Xu, C., Kobata, K., Andersen, M., Barker, S., Yu, J., and Foster, G.: Continuous CO2 reconstruction across the MPT from boron isotopes informs mechanisms of glacial CO2 change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20791, https://doi.org/10.5194/egusphere-egu26-20791, 2026.

EGU26-20885 | ECS | Posters on site | CL1.2.8

Inferring climate variability from replicated Antarctic ice-core water isotope records 

Kathrin Brocker, Thom Laepple, Maria Hörhold, Hanno Meyer, Frank Wilhelms, Melanie Behrens, Johannes Freitag, Daniela Jansen, Ilka Weikusat, Hans-Christian Steen-Larsen, Nora Hirsch, and Amaëlle Landais and the Beyond-EPICA isotope consortium

Changes in climate variability are as critical to understand as changes in the mean climate, yet remain difficult to quantify from ice cores because single records are strongly affected by local noise arising from depositional, post-depositional, and diffusive processes. As a result, past changes in climate variability cannot be robustly separated from changes in ice-core noise using individual cores alone.
This limitation can be overcome by analysing replicated ice-core records, where the common signal can be interpreted as climate-driven variability. For the first time, such an approach is now feasible for deep Antarctic ice cores through the paired water-isotope records of EPICA Dome C and the new Beyond EPICA Oldest Ice Core (BE-OIC), which together provide a replicated archive extending back 800,000 years.
Here, we present first results from the upper ~ 300 m of the BE-OIC ice core focusing on Holocene variability in stable water isotopes. Using spectral methods, we compare the statistical properties of isotope variability between the two cores to separate common climate variability from local noise and to assess the effective temporal resolution of the preserved signal. These preliminary results provide an initial step towards quantifying multidecadal to millennial-scale climate variability in Antarctic temperature during the Holocene and establish the basis for extending this analysis to earlier interglacial periods with the BE-OIC ice core record.

How to cite: Brocker, K., Laepple, T., Hörhold, M., Meyer, H., Wilhelms, F., Behrens, M., Freitag, J., Jansen, D., Weikusat, I., Steen-Larsen, H.-C., Hirsch, N., and Landais, A. and the Beyond-EPICA isotope consortium: Inferring climate variability from replicated Antarctic ice-core water isotope records, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20885, https://doi.org/10.5194/egusphere-egu26-20885, 2026.

Oxidation products of biogenic volatile organic compounds, such as monoterpenes and isoprene, are widely used to investigate variability in biogenic emissions and atmospheric transformation processes. Quantifying such tracers in ice-core matrices remains challenging because concentrations are ultralow and results can be affected by matrix effects and contamination. Here, we developed a targeted ultratrace LC–MS³ method using a SCIEX QTRAP 5500+ to enhance sensitivity and selectivity for five established SOA markers: cis-pinonic acid, pinic acid, keto-pinic acid, 3-methyl-1,2,3-butanetricarboxylic acid (3-MBTCA), and 2-methylerythritol (2-ME). Method performance was evaluated using procedural blanks and spike-recovery experiments, yielding compound-specific reporting limits of 0.01–0.05 ppt (limits of detection, LOD) and 0.1–0.25 ppt (limits of quantification, LOQ); instrument repeatability based on batch quality-control injections was 5–8% RSD.

The method was applied to meltwater fractions from the oldest section (>700,000 years ago) of the Beyond EPICA ice-core collected sequentially within each core section, resulting in 878 analysed fractions from 183 sections spanning 2399.0–2581.8 m (≈0.66 to ≥1.47 Ma BP, modelled). Concentrations are reported as ppt in meltwater following direct analysis (no preconcentration). Pinic acid was detected above the LOD in 87% of analysed fractions and quantified above the LOQ in 62%, with concentrations ranging from 0.87 to 5.83 ppt (mean 2.19 ppt). 3-MBTCA was detected in 70% of fractions and quantified in 66%, with concentrations of 0.103–0.612 ppt (mean 0.196 ppt). In contrast, cis-pinonic acid and 2-ME were below the LOQ, 0.1 ppt, while keto-pinic acid was not detected in the analysed ice-core samples.

These first measurements, placed within a preliminary age framework, demonstrate quantification of biogenic SOA tracers in Beyond EPICA ice-core at ultratrace levels. Ongoing work will integrate these data with co-measured glaciochemical tracers to evaluate transport, deposition and post-depositional effects, and to assess the potential of these compounds as proxies for past biogenic emissions and atmospheric oxidative processing.

How to cite: Kolawole, T. and the Beyond EPICA: Temporal variability of ultratrace biogenic secondary organic aerosol markers in the oldest ice from Beyond EPICA, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21228, https://doi.org/10.5194/egusphere-egu26-21228, 2026.

EGU26-21616 | Posters on site | CL1.2.8

Visual stratigraphy of the BEOIC oldest-ice section – preliminary results from linescan images 

Johannes Freitag, Daniela Jansen, Ilka Weikusat, Nicolas Stoll, Julien Westhoff, Maria Hörhold, Melanie Behrens, and Frank Wilhelms

During the main BEOIC processing campaign in 2025 at AWI, linescan images of double-sided polished ice slabs were routinely recorded. The linescanner is a well-established optical system in ice-core analysis that operates in darkfield mode, capturing scattered light from internal reflection surfaces and nuclei that are mostly associated with dust particles within the ice. The spatial resolution of the images is in the sub-millimetre range. As the measurement method produces almost no signal dispersion, it enables an exceptionally detailed view of small-scale layering.

In this contribution, we present images and grey-value records of the oldest-ice section between 2400 m and 2580 m depth and provide a preliminary interpretation of the observed features. Owing to the expected strong thinning—where more than 10,000 years may be compressed into a single metre of ice—these data offer a first indication of the limits of temporal resolution that can be achieved with other proxy parameters. Further image analysis addresses ice deformation as well as questions of stratigraphic integrity and continuity at the BEOIC site. We focus on selected depth intervals and present an initial overview of the evolution of lateral stability in the layered structures observed in the data.

How to cite: Freitag, J., Jansen, D., Weikusat, I., Stoll, N., Westhoff, J., Hörhold, M., Behrens, M., and Wilhelms, F.: Visual stratigraphy of the BEOIC oldest-ice section – preliminary results from linescan images, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21616, https://doi.org/10.5194/egusphere-egu26-21616, 2026.

EGU26-22482 | Posters on site | CL1.2.8

Windblown diatoms at Little Dome C and their potential for reconstructing Southern Hemisphere Westerly Winds during the MPT  

Dieter Tetzner, Claire Allen, Delia Segato, James Veale, Romilly Harris-Stuart, and Julien Westhoff

The Southern Hemisphere Westerly Winds play a crucial role in the Earth's climate system and may have influenced the physical and biological processes that drove CO2 exchange in the Southern Ocean during the Mid-Pleistocene Transition (MPT). Numerous paleoclimate archives have been utilised to reconstruct past westerly winds over different timescales; however, many are limited by their reliance on precipitation or temperature proxies to infer SHWW changes. Marine diatoms found in Antarctic ice core layers have recently established as a reliable proxy for directly reconstructing historical changes in wind strength and atmospheric circulation within the Southern Hemisphere Westerly Wind belt.

In this study, we present diatom records preserved in two snow pits from Little Dome C and in Holocene samples from the EPICA Dome C ice core. The annual abundance of diatoms preserved in Little Dome C snow layers strongly correlates with wind strength over South America and the South Atlantic sector of the Southern Ocean. Backward trajectory analyses enable us to trace the pathways of air masses before reaching the Little Dome C site, aiming to identify potential primary source regions for the Little Dome C diatoms. The strong positive correlation between Little Dome C diatoms and wind strength in South America and the South Atlantic highlights the potential to use diatoms preserved in the BE-OI as a proxy for reconstructing past changes in mid-latitude winds. This study lays the groundwork for further exploration of diatom records preserved in excess meltwater collected during the BE-OI slow CFA campaign.

How to cite: Tetzner, D., Allen, C., Segato, D., Veale, J., Harris-Stuart, R., and Westhoff, J.: Windblown diatoms at Little Dome C and their potential for reconstructing Southern Hemisphere Westerly Winds during the MPT , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22482, https://doi.org/10.5194/egusphere-egu26-22482, 2026.

CR6 – Instrumental and paleo-archive observations, analyses, and data-driven methods in the cryospheric sciences

EGU26-364 | ECS | Orals | CR6.1

Beyond Teleconnections - Uncovering Stable Drivers of Antarctic Sea Ice Anomalies 

Nina Susann Öhlckers, Dirk Lorenz, and Monica Ionita

Antarctic Sea Ice (ASI) has experienced a sudden and drastic decline since 2016, following decades of gradual growth since the start of satellite observations. This sharp reversal caused suggestions that a regime shift has happened. However, the underlying drivers remain uncertain due to complex atmosphere-ocean interactions and pronounced regional variability. While atmospheric circulation patterns and large-scale teleconnections influence ASI variability, their spatial aggregation limits their ability to explain regional changes. Recent studies point to an increasing role of ocean heat content, yet its contribution relative to atmospheric influences has not been quantified. In this study, we address this gap by developing a framework to identify stable, spatially coherent climate drivers of regional ASI. We first introduce a workflow combining correlation analysis with HDBSCAN clustering to detect global clusters that have persistent correlations with regional ASI and can serve as robust predictors. We then use these clusters as input features in a linear regression model combining atmospheric variables and ocean heat content to assess how well ASI variability can be reconstructed. Finally, we evaluate how the relative importance of atmospheric and oceanic drivers has changed before and after the extreme low-ice events beginning in 2016.

Our results demonstrate that (1) the proposed clustering framework reliably identifies physically meaningful driver regions, (2) a linear model using these drivers can successfully reproduce regional ASI variability, and (3) the contribution of ocean heat relative to atmospheric forcing varies markedly across regions.

How to cite: Öhlckers, N. S., Lorenz, D., and Ionita, M.: Beyond Teleconnections - Uncovering Stable Drivers of Antarctic Sea Ice Anomalies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-364, https://doi.org/10.5194/egusphere-egu26-364, 2026.

EGU26-518 | ECS | Orals | CR6.1

Efficient Sea Ice Classification Built on Few-Shot Learning Framework 

yang li, Petteri Uotila, Chao Li, Matti Leppäranta, and Chongtai Peng

Deep learning (DL) methods have become a key technique for automatic sea ice type mapping from synthetic aperture radar (SAR) imagery, yet their deployment in operational sea ice charting is still hindered by scarce labelled data, limited adaptive feature extraction, and the lack of interactive mechanisms, which restrict model generalization, accuracy, and usability, especially in hard-to-classify scenes. To address these bottlenecks, we propose an efficient sea ice classification model, ESICM, targeting four ice types: open water (OW), young ice (YI), first-year ice (FYI), and multiyear ice (MYI), and enhance performance and practicality under label-scarce conditions through three key designs. First, we introduce a few-shot learning (FSL) framework to more effectively exploit limited labels and reduce the reliance of traditional supervised learning on large labelled datasets. Second, inspired by classical sea ice parameter retrieval algorithms, we design a lightweight channel multiply–divide convolution module (CMDM) that strengthens adaptive feature extraction with only ~190k parameters, thereby improving discrimination of multi-scale textures and sea ice types with subtle backscattering differences. Third, we incorporate an interactive mechanism based on the Segment Anything Model (SAM) and couple it with the FSL framework, allowing the classifier to be adjusted with minimal human intervention and thus improving operability in difficult SAR scenes. ESICM is trained on 512 scenes from the AI4Arctic sea ice challenge dataset and evaluated on 20 independent test scenes, achieving 91.73% overall accuracy (OA), 91.29% F1 score, 85.61% Cohen’s kappa, and 71.52% mean intersection over union (mIoU), outperforming comparative DL models by at least 1.35, 1.90, 2.54, and 2.53 percentage points on these metrics, respectively. In melting season scenes, particularly those dominated by MYI, ESICM’s F1 and IoU outperform the second-best model by 22.21% and 19.15%, respectively. Further cross-domain experiments demonstrate that, even when trained on only about one quarter of local scenes, ESICM still achieves the highest accuracy, demonstrating strong cross-regional generalization. Meanwhile, its interactive functionality enables users to refine classification results via prompts in hard-to-classify scenes, substantially enhancing classification performance. Overall, ESICM provides a lightweight, high-accuracy, and interactively adjustable DL solution for SAR-based sea ice classification under limited labelled data, offering robust technical support for polar navigation safety and sea ice environmental monitoring.

How to cite: li, Y., Uotila, P., Li, C., Leppäranta, M., and Peng, C.: Efficient Sea Ice Classification Built on Few-Shot Learning Framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-518, https://doi.org/10.5194/egusphere-egu26-518, 2026.

EGU26-1379 | ECS | Orals | CR6.1

Mapping the Margins: Evaluating Accuracy and Ambiguity in Automated Rock Glacier Delineation 

Sunil Tamang, Shelley MacDonell, James Brasington, James Shulmeister, and Benjamin Aubrey Robson

Rock glaciers, the most visible surface expression of permafrost landforms, are found across glacial, periglacial and paraglacial environments. Accurate and consistent mapping of their extent is fundamental for advancing research in geomorphology, hydrology, ecology, geohazard assessment, permafrost dynamics, and climate studies. However, delineating their boundary remains challenging because rock glaciers often occur alongside or merge with other geomorphic equifinal landforms that are difficult to distinguish by their spectral identity in aerial or satellite imagery. Additionally, their boundaries are inherently ambiguous, evolving with changes in topographic and climatic factors. The widely used approach involving manual digitisation through visual interpretation of geomorphic features is time-consuming and subjective. Recent studies have explored deep learning as a means to automate and scale up rock glacier mapping, but existing studies still remain limited in number and geographic scope, with minimal attention to evaluating discrepancies or uncertainties in mapped extents.  This study examines the use of a U-Net deep learning model for automated delineation of rock glacier extent, with particular emphasis on associated uncertainties. Using data from the Chile National Glacier Inventory for the Coquimbo region, we trained the model under two strategies: (1) differentiated training based on rock glacier types. A set of models was trained exclusively on landforms with clearly expressed geomorphological features of frontal slopes, lateral margin, and ridge-furrow structures, while another set incorporated all inventoried rock glaciers, including both well-expressed and subdued geomorphological features; (2) different predictor combinations, comparing a configuration that used only RGB + NIR bands from Sentinel 2 or PlanetScope imagery with an expanded set that integrated these spectral bands with DEM derivatives and imagery-derived variables.  The highest-performing models from these strategies were then applied to an independent test area, and their outputs were compared against existing inventories to evaluate spatial consistency and assess potential mapping biases. By integrating an automated method with uncertainty assessment, this work contributes to the ongoing advancement of rock glacier detection and delineation methods and highlights the critical need to validate deep learning outputs. Such uncertainty quantification is essential for ensuring the robustness of mapped extents and for supporting applications that depend on accurate and reliable representations of landforms with inherently ambiguous and dynamic boundaries.

How to cite: Tamang, S., MacDonell, S., Brasington, J., Shulmeister, J., and Robson, B. A.: Mapping the Margins: Evaluating Accuracy and Ambiguity in Automated Rock Glacier Delineation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1379, https://doi.org/10.5194/egusphere-egu26-1379, 2026.

EGU26-3470 | ECS | Posters on site | CR6.1

Mapping “cold spots” of potential hidden alpine permafrost using semi-supervised machine learning 

Yaniv Goldschmidt, Jacopo Boaga, and Francesco Marra

Geophysical techniques revealed frozen ground within relict periglacial landforms in which the presence of ice was excluded by traditional geomorphological and topographic approaches. These unexpected frozen bodies, referred to here as cold spots, suggest that permafrost can exist outside traditionally mapped permafrost zones. Under climate change, with retreating glaciers and increasing snow variability, subsurface ice in periglacial landforms becomes a potentially important but overlooked water resource. However, its spatial distribution and climatic controls remain poorly understood.

Here, we develop a methodology to identify cold spots. We focus on the Southern Alps and we assume that cold spots are related to micro-climatic and topographic conditions that allow permafrost to persist. We use a limited set of sites investigated by geophysical surveys, including confirmed cold spots and geomorphologically similar control sites without permafrost. We analyze topographic and climatic remote-sensing data to derive relevant features and examine their relation to cold spots. We then use these features in semi-supervised machine learning classification models to identify areas with conditions similar to known cold spots. The resulting maps highlight potential cold-spot locations targeted for forthcoming geophysical field investigations and provide a practical framework for improving the detection of hidden permafrost.

How to cite: Goldschmidt, Y., Boaga, J., and Marra, F.: Mapping “cold spots” of potential hidden alpine permafrost using semi-supervised machine learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3470, https://doi.org/10.5194/egusphere-egu26-3470, 2026.

EGU26-7803 | ECS | Orals | CR6.1

Self-supervised learning reduces labelling requirements for sea ice segmentation in Sentinel-1 SAR imagery  

Jacob Seston, William D. Harcourt, Georgios Leontidis, Brice Rea, Matteo Spagnolo, and Lauren McWhinnie

Monitoring Arctic sea ice variability is crucial for maritime safety. Synthetic Aperture Radar (SAR) imagery provides an effective means of achieving this through all-weather, day-and-night coverage of the Arctic. Navigation in the Canadian Arctic Archipelago currently relies on operational ice information services, including analyst-derived ice charts, satellite imagery, and ice routing products provided by national ice services However, the development of machine-learning systems capable of automatically processing large volumes of satellite imagery and accurately identifying ice conditions is constrained by the need for extensive manually labelled datasets. To address this limitation, we developed a self-supervised learning (SSL) approach, which uses unlabelled data to learn general image representations. Specifically, we use Bootstrap Your Own Latent (BYOL), a non-contrastive SSL framework, to pretrain a UNet encoder on unlabelled dual-polarised Sentinel-1 Extra-Wide mode (EW) SAR scenes before fine-tuning with a small set of labelled images. We compare the BYOL-pretrained UNet (called UNet SSL in this study) to four baselines: a control UNet, a fully supervised UNet, a Random Forest classifier, and the Segment Anything Model (SAM). With only three labelled scenes, the BYOL-pretrained UNet achieved higher segmentation accuracy than the fully supervised model trained on seven images, more than twice the number of labelled scenes. The most significant gains occurred in Marginal Ice Zone (MIZ) scenes, where the BYOL-pretrained UNet achieved a Matthews Correlation Coefficient  (MCC) of 0.2087, compared with 0.1685 for the fully supervised UNet trained on seven labelled scenes and 0.1449 for the control model trained on three scenes—representing an MCC increase of approximately 24% and 44%, respectively. These improvements were accompanied by a substantial reduction in false negatives and a marked increase in recall, indicating improved discrimination under low-contrast, fragmented floe conditions. Our findings demonstrate that SSL reduces annotation requirements for SAR-based sea ice segmentation, improving model generalisation in both consolidated and fragmented ice conditions. This approach offers a scalable solution to the labelling bottleneck in Arctic monitoring and highlights the potential of BYOL as a general pretraining strategy for SAR-based Earth observation image segmentation. 

How to cite: Seston, J., Harcourt, W. D., Leontidis, G., Rea, B., Spagnolo, M., and McWhinnie, L.: Self-supervised learning reduces labelling requirements for sea ice segmentation in Sentinel-1 SAR imagery , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7803, https://doi.org/10.5194/egusphere-egu26-7803, 2026.

EGU26-8748 | ECS | Posters on site | CR6.1

Seasonal Predictability of Antarctic Sea Ice based on Deep-learning Approach 

Gyeongmin Baek, Jiho Ko, Emilia Kyung Jin, and Jong-Seong Kug

There is a distinct difference in the behavior of sea ice extent response to global warming between the Arctic and Antarctic; the former is decreasing while the latter had been increasing slightly until recently. However, satellite data show that Antarctic sea ice has been continuously decreasing since 2016 and reached its minimum in February 2023. The minimization of sea ice extent in Antarctica would have various impacts on the Earth's system. Since ice is more reflective than liquid water, sea ice plays a significant role in maintaining the Earth’s energy balance. Therefore, it is crucial to accurately predict future sea ice response. Here, we aim to predict the sea ice extent for the upcoming season using deep learning models, employing U-Net. Atmospheric and oceanic data related to sea ice, such as sea surface temperature, wind speed, etc., were used as features, while the sea ice extent was set as the target. We trained and tested the models using data from the CESM2 Large Ensemble. We tarined the final model by fine-tuning the model pre-trained on numerical model data with observational data. The performance of the models was compared using ACC and RMSE as evaluation metrics. Additionally, to assess the impact of each variable within the model, we replaced each variable with its climatological mean and observed the changes in the evaluation metrics to determine their importance. These research findings are anticipated to significantly contribute to predicting more accurate changes in Antarctic sea ice and understanding future Antarctic sea ice changes.

 

How to cite: Baek, G., Ko, J., Jin, E. K., and Kug, J.-S.: Seasonal Predictability of Antarctic Sea Ice based on Deep-learning Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8748, https://doi.org/10.5194/egusphere-egu26-8748, 2026.

EGU26-9225 | ECS | Orals | CR6.1

A machine-learning-based super-resolution approach for dynamical ice-sheet modeling 

Sebastian Scher, Andy Aschwanden, Florina Schalamon, Andreas Trügler, and Jakob Abermann

Dynamical ice-sheet models are among the primary tools used to investigate the evolution of ice sheets. However, their computational cost increases rapidly with spatial resolution, often making long-term or ensemble simulations prohibitively expensive. Here, we investigate whether recent advances in machine-learning-based super-resolution techniques for spatiotemporal data can be leveraged to reduce these computational costs while retaining high-resolution information.

Using one pair of low- and high-resolution simulations of the Greenland ice sheet for the 20th century, generated with the PISM dynamical ice-sheet model, we train a machine-learning-based super-resolution model to learn the mapping from low- to high-resolution states. For subsequent simulations, computationally inexpensive low-resolution model runs are combined with the trained super-resolution model to reconstruct high-resolution fields. We evaluate this hybrid framework by assessing (1) whether the super-resolution model can accurately reproduce the spatial details of high-resolution simulations, and (2) whether it can mitigate deficiencies in the long-term trends produced by low-resolution models. Our results provide insight into the potential of machine-learning-based super-resolution as a cost-effective tool for high-resolution dynamical ice-sheet modeling.

How to cite: Scher, S., Aschwanden, A., Schalamon, F., Trügler, A., and Abermann, J.: A machine-learning-based super-resolution approach for dynamical ice-sheet modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9225, https://doi.org/10.5194/egusphere-egu26-9225, 2026.

EGU26-10587 | ECS | Posters on site | CR6.1

Exploring machine-learning extrapolation of glacier elevation change in High Mountain Asia derived from ICESat-2 data 

Ying Huang, Lei Huang, and Tobias Bolch

Glacier elevation change is a fundamental measure for quantifying glacier mass balance and assessing glacier–climate interactions. Large-scale estimates are commonly derived either from satellite altimetry, which provides robust but spatially sparse measurements, or from digital elevation model (DEM) differencing, which enables spatially continuous mapping but is more sensitive to noise and bias in complex mountain terrain. Machine learning (ML) approaches have increasingly been used to bridge this gap by correcting or reconstructing elevation measurements using climate and topographic predictors. However, because ML-based prediction inherently involves extrapolation beyond directly sampled glaciers, its reliability across heterogeneous glacier systems such as existing in High Mountain Asia (HMA)remains poorly constrained.

In this study, we explore the behaviour of ML-based glacier elevation change predictions trained with ICESat-2 elevation measurements combined with climate and terrain variables across multiple HMA subregions. ICESat-2 footprints provide dense elevation change observations over only a limited subset of glaciers within each subregion. We train subregion-specific XGBoost models and evaluate their performance in relation to glacier sampling characteristics, feature importance, and elevation-dependent behavior.

The results reveal pronounced regional contrasts despite comparable glacier size and sample coverage across regions. In the Karakoram for example, ML-based extrapolation produces spatially coherent and elevation-dependent patterns of glacier elevation change, with predicted dh systematically decreasing from lower to higher elevations, consistent with expected glacier-scale behavior. These structured predictions are associated with robust model performance (R² ≈ 0.7). In contrast, in West Kunlun Shan, extrapolated elevation change fields are spatially uniform and weakly structured, showing little sensitivity to the applied climate and terrain predictors. These results indicate that the effectiveness of ML-based glacier elevation change modeling depends less on sample size or glacier extent alone than on the presence of stable and internally consistent response structures within glacier systems.

How to cite: Huang, Y., Huang, L., and Bolch, T.: Exploring machine-learning extrapolation of glacier elevation change in High Mountain Asia derived from ICESat-2 data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10587, https://doi.org/10.5194/egusphere-egu26-10587, 2026.

EGU26-12034 | ECS | Orals | CR6.1

Creating a high-resolution Northern Hemisphere daily SWE dataset (1980-2020) using Machine Learning 

Oriol Pomarol Moya, Derek Karssenberg, Walter W. Immerzeel, Philip Kraaijenbrink, Madlene Nussbaum, and Siamak Mehrkanoon

Snow water equivalent (SWE) is an important component of the global hydrological cycle, acting as a primary reservoir for seasonal water storage. Despite its relevance, only few datasets are available that provide long-term daily SWE estimates at global scale. Even amongst the best gridded SWE products, the spatial resolution does not go beyond 10km, a significant limitation considering the large spatial variability of snow. Furthermore, assimilation of snow observations in such products remains another key challenge. Machine learning (ML) models and their combination with process-based simulations, what is known as Hybrid Modelling, offer a promising alternative for producing detailed SWE predictions at large scales, given their high inference speed and adaptability to their training data. Hybrid ML models have already been used for SWE prediction over a small number of sites, improving both pure ML approaches and advanced process-based snow models such as Crocus, but their applicability for long-term spatiotemporal modelling of snow at larger scales remains to be tested.

In this project, we trained an LSTM model using in-situ snow data from roughly 10000 sites throughout the Northern Hemisphere with the aim of creating a 40-year gridded dataset of daily SWE at 1 km resolution. The model incorporates temperature, precipitation, and shortwave radiation as meteorological predictors, alongside a small set of topographic variables and land cover classification. Preliminary results show a good fit to stations excluded from the training set, with an RMSE of 44 mm, where unequal distribution of observation locations was accounted for by a weighting scheme. These findings suggest the suitability of this approach for extending coverage to ungauged regions across the Northern Hemisphere. The use of the ERA5-Land SWE product as a hybrid support promises further improvements in model performance.

Ultimately, this project aims to provide a finer-scale alternative to existing daily SWE products. By improving the spatial resolution to 1km and incorporating available snow measurements, it contributes to a more refined view of seasonal snow storage across the Northern Hemisphere.

How to cite: Pomarol Moya, O., Karssenberg, D., Immerzeel, W. W., Kraaijenbrink, P., Nussbaum, M., and Mehrkanoon, S.: Creating a high-resolution Northern Hemisphere daily SWE dataset (1980-2020) using Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12034, https://doi.org/10.5194/egusphere-egu26-12034, 2026.

EGU26-12303 | Posters on site | CR6.1

Hybrid training for robust emulator-based ice-thickness inversion 

Sebastian Rosier, Thomas Gregov, Brandon Finley, Guillaume Jouvet, and Andreas Vieli

Ice-flow inversions aim to infer unobserved controls on glacier and ice-sheet dynamics from limited, noisy surface data but are notoriously ill-posed: multiple parameter fields can reproduce the same observations, solutions are sensitive to priors/regularization, and model nonlinearity amplifies both data and structural errors. Here we target a particularly challenging variant — emulator-based inversion using a machine-learning surrogate for ice flow — where the forward operator is fast and differentiable but only an approximation of the governing physics. We focus on inverting for ice thickness, which remains poorly constrained for most glaciers yet strongly conditions driving stress, basal traction, and therefore hindcast skill and projection uncertainty.

We present emulator-based inversions with the Instructed Glacier Model (IGM), benchmarking against synthetic tests with known truth and contrasting performance with a full-physics ice-flow solver. IGM provides a PINN-based emulator trained by minimizing a energy representing the Blatter–Pattyn equations. This powerful approach has proven very successful in the forward problem but leads to an emulator that may need regular retraining to ensure an accurate solution. We show that this training approach can introduce surrogate error modes that distort gradients and create spurious minima, degrading convergence and reliability of gradient-based optimization used for the inverse problem. To address this, we introduce a hybrid training strategy that augments the physics loss with a data-misfit term against a large training set, with the aim of improving out-of-distribution generalization across glacier geometries. The resulting emulator yields more reliable recovery of unknown fields such as ice thickness and supports the fast, scalable inversions needed for ensemble modelling and robust uncertainty quantification.

How to cite: Rosier, S., Gregov, T., Finley, B., Jouvet, G., and Vieli, A.: Hybrid training for robust emulator-based ice-thickness inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12303, https://doi.org/10.5194/egusphere-egu26-12303, 2026.

EGU26-13166 | ECS | Posters on site | CR6.1

A Random Forest and XGBoost analysis of the temporal and spatial variability of snow depth in the Zugspitze region based on terrain features, simulated energy balance and remote sensing 

Paul Schattan, Jakob Knieß, Simon Gascoin, Juilson Jubanski, Roberta Facchinetti, Carolin Rempfer, Karl-Friedrich Wetzel, Christian Voigt, Karsten Schulz, and Franziska Koch

Temporal and spatial patterns of snow depth are key predictors for variations in snow water equivalent and snow-hydrological processes. Observations of snow depth distribution are usually scarce either in space or in time. Automatic weather stations can measure snow depth continuously but only for one point with a very small footprint. Campaign based surveys, in contrast, cover larger areas but are limited in spatial coverage due to technical and logistical constraints.

The partial recurrence of snow depth patterns correlated with terrain features is well known. In this work a machine learning approach based on Random Forest and XGBoost is presented to analyze the temporal evolution of snow depth distributions in the Zugspitze region. Input features include elevation and derived terrain features like slope, aspect, curvature, topographic position index and Winstral wind shelter index. Furthermore, simulated energy balance sums and snow occurrence from optical remote sensing data are used. Snow depth data include terrestrial Lidar measurements and photogrammetric data based on airborne and spaceborne platforms including drones, airplanes and the Pléiades satellite constellation.

Interestingly, due to the specific topography of the area featuring a karstic plateau surrounded by steep slopes, no clear elevational gradients were found. Historical information constitutes a useful feature for machine learning but explains only parts of the variability as actual snow depth distributions are altered by wind drift and energy balance. This is reflected by a moderate temporal transferability of the trained machine learning models. Within the study domain, campaign specific machine learning models produce plausible results for areas with data gaps. While Random Forest and XGBoost produce similar results, differences between different sets of input features can be substantial. Meltout patterns based on remote sensing data can partly compensate for a lack of historical snow depth information.

Machine learning proves to be a suitable tool for closing spatial data gaps. The results also highlight the importance of a process-based choice of input features, as inter- and intraannual snow depth distributions differ even in a region with stable snow depth patterns.

How to cite: Schattan, P., Knieß, J., Gascoin, S., Jubanski, J., Facchinetti, R., Rempfer, C., Wetzel, K.-F., Voigt, C., Schulz, K., and Koch, F.: A Random Forest and XGBoost analysis of the temporal and spatial variability of snow depth in the Zugspitze region based on terrain features, simulated energy balance and remote sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13166, https://doi.org/10.5194/egusphere-egu26-13166, 2026.

EGU26-13443 | ECS | Orals | CR6.1 | Highlight

Icebergs as a Distributed Sensor Network: Iceberg Tracking in Time-Lapse Imagery for Fjord Circulation Analysis 

Marco Jaeger-Kufel, Anja Neumann, Andreas Vieli, Andrea Kneib-Walter, Ethan Welty, and Josefine Umlauft

Tidewater glaciers are critical gateways for global sea level rise, with their stability strongly influenced by complex fjord circulation patterns that control submarine melting. Direct observations of these dynamics with conventional oceanographic instruments remain challenging due to temporal or spatial constraints. However, the fjords themselves contain a distributed sensor network: icebergs. As passive tracers driven by currents, icebergs of different sizes respond to circulation at different depths due to their varying underlying drafts. Deriving quantitative circulation data from these tracers requires tracking hundreds to thousands of similar-looking icebergs simultaneously.

This work presents an automated multi-object-tracking framework that extracts dense, size-stratified velocity fields from time-lapse imagery, providing the observational foundation required to reconstruct depth-dependent circulation patterns within glacier fjords. We introduce a scale-adaptive object detection architecture based on Faster R-CNN that achieves 87.1\% detection recall and successfully captures a large fraction of the iceberg population from only a sparse set of manual labels. To maintain persistent identities in dense scenes, we employ a multi-modal association strategy that combines Kalman-filtered motion priors with appearance similarity learned via Vision Transformers. Evaluated across diverse environmental conditions, the framework demonstrates high stability with 95.7\% identity consistency (IDF1) at 2-minute time intervals and generalizes to unseen glaciers without retraining. By transforming time-lapse imagery into quantitative circulation records, this work provides a robust framework for monitoring the hidden ocean dynamics that drive glacier retreat.

How to cite: Jaeger-Kufel, M., Neumann, A., Vieli, A., Kneib-Walter, A., Welty, E., and Umlauft, J.: Icebergs as a Distributed Sensor Network: Iceberg Tracking in Time-Lapse Imagery for Fjord Circulation Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13443, https://doi.org/10.5194/egusphere-egu26-13443, 2026.

EGU26-14626 | ECS | Orals | CR6.1

From seismic signals to calving drivers: Assessing twelve years of glacial earthquakes in Greenland using Random Forest models 

Selina Wetter, Anne Mangeney, Eléonore Stutzmann, Clément Hibert, and Stuart N. Lane

Quantifying iceberg calving is important for understanding ice mass loss of the Greenland Ice Sheet and its subsequent impact on sea level rise, and for refining calving laws that currently represent a major source of uncertainty in global climate models. These calving events, particularly those involving capsizing icebergs, exert time-varying forces on the edge of marine-terminating glaciers that produce distinct seismic signals known as glacial earthquakes.

By processing twelve years of continuous seismic data and employing a Random Forest classifier to distinguish these glacial earthquakes from tectonic events, we generated a comprehensive catalogue of 6263 previously undocumented glacial earthquakes occurring between 2013 and 2024. The detected events are located along the Greenland coast with surface wave magnitudes ranging from MSW 4.1 to 5.4. They cluster at nine major calving glaciers, though the vast majority of activity is concentrated at Sermeq Kujalleq (Jakobshavn Isbræ) and Helheim Gletsjer.

To investigate the driving mechanisms behind these events, we analysed the correlation between calving activity and various environmental variables, including glacier velocity, air temperature, sea ice fraction, sea surface temperature, and wind speed. We train a second Random Forest model to predict monthly calving events and evaluate the relative importance of these environmental features, while applying statistical analyses to investigate correlations on a yearly basis where data points are limited. Our results indicate that the relationship between calving and the environment is highly complex and site-specific, as no single variable serves as a universal driver for all glaciers.

This complexity is further highlighted by scale-dependent correlations between calving events and environmental variables. For instance, while the glacier velocity shows a strong correlation with cumulative yearly calving at Sermeq Kujalleq, its importance diminishes on a monthly scale. Conversely, Helheim Gletsjer exhibits no clear yearly correlation with the glacier velocity, highlighting the site-specific nature of calving dynamics. We will present the spatio-temporal evolution of the detected events and discuss how these diverse environmental correlations quantify the varying sensitivity of individual glaciers to environmental forcing across different temporal scales.

How to cite: Wetter, S., Mangeney, A., Stutzmann, E., Hibert, C., and Lane, S. N.: From seismic signals to calving drivers: Assessing twelve years of glacial earthquakes in Greenland using Random Forest models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14626, https://doi.org/10.5194/egusphere-egu26-14626, 2026.

EGU26-15167 | Posters on site | CR6.1

Quantifying the uncertainty of regime shifts in the paleoclimate via physics-informed emulation and expert knowledge 

Dimitra Salmanidou, Lauren Gregoire, Brooke Snoll, Charli Frisby, Matt Graham, and Serge Guillas

The absence of data in the existing instrumental record significantly limits our ability to comprehend and forecast tipping points in the Greenland Ice Sheet (GrIS) and Subpolar Gyre (SPG). Multidirectional approaches are therefore required to capture the complexity of systemic changes and support future early warning efforts. In this study we discuss the ongoing work of the research project VERIFY: Out Of Sample Testing For Early Warning Systems Using Past Climate. We combine computational experiments, with physics-informed emulation and insights from expert elicitation to better understand dirvers of paleoclimate regime shifts in the GrIS. Employing uncertainty quantification methods, we make use of machine learning surrogate models to approximate the system's response. Surrogate models can accurately mimic input-output relationships of complex and computationaly expensive models, providing the opportunity to produce large ensembles for fully exploring the range of plausible model inputs. The goal is to understand what drives the exceedance of critical thresholds through the integration of computational experiments, machine learning and current scientific knowledge.

How to cite: Salmanidou, D., Gregoire, L., Snoll, B., Frisby, C., Graham, M., and Guillas, S.: Quantifying the uncertainty of regime shifts in the paleoclimate via physics-informed emulation and expert knowledge, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15167, https://doi.org/10.5194/egusphere-egu26-15167, 2026.

EGU26-16321 | ECS | Posters on site | CR6.1

A Lightweight Hybrid CNN–Transformer Architecture for High‑Resolution Downscaling and Bias Correction of Snow Water Equivalent 

Mubashshir Ali, Farid Ait-Chaalal, Siddharth Kumar, and Alison Dobbin

Accurate, high‑resolution Snow Water Equivalent (SWE) information is critical for reliable hazard assessment and effective water resource management. Yet, widely used global reanalysis products provide SWE at coarse spatial scales and exhibit substantial terrain‑ and melt‑related biases. In contrast, dynamically downscaled products offer improved detail but are costly to run and thus, remain limited in availability.

To address this limitation, we introduce the Linear Attention Snow Downscaling Model (LASDM), a lightweight hybrid deep learning architecture designed specifically to enhance the spatial detail and physical realism of SWE fields. LASDM combines convolutional neural networks with linear attention based transformer blocks, enabling efficient representation of synoptic‑to‑local snow processes while remaining highly parameter‑efficient (<1 million parameters).

Applied to the ERA5 → ERA5‑Land downscaling problem over the Great Lakes region (1980–2022), LASDM demonstrates stronger performance than U‑Net, Swin Transformer, and statistical baselines across a range of evaluation metrics. Case studies for two winter storms provide additional context for these differences. More broadly, this work suggests the potential of machine‑learning architectures for downscaling and bias correction. LASDM offers a compact and adaptable framework that may help improve snow representation and support applications that rely on higher‑resolution SWE.

How to cite: Ali, M., Ait-Chaalal, F., Kumar, S., and Dobbin, A.: A Lightweight Hybrid CNN–Transformer Architecture for High‑Resolution Downscaling and Bias Correction of Snow Water Equivalent, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16321, https://doi.org/10.5194/egusphere-egu26-16321, 2026.

EGU26-16558 | ECS | Posters on site | CR6.1

Enhancing sea ice concentration prediction with multi-task learning and conditional residual refinement 

Woohyeok Kim, Inchae Chung, Ga-ryung Lee, Minki Choo, and Jungho Im

Sea ice covers the oceans in polar regions and is closely related to heat circulation between the Sun and the Earth, and the absolute amount of sea ice can represent climate change itself. The research aiming to prepare for future climate conditions by predicting sea ice concentration (SIC), the area ratio of the ocean covered by sea ice, is being actively conducted.

From a long-term perspective, sea ice is influenced by sea surface temperature (SST), 2 m air temperature (t2m), wind fields, and so on, and machine learning or deep learning techniques are used to predict SIC in order to leverage the correlations among variables. However, due to the characteristics of deep learning techniques, there are limitations in identifying how much each variable influences the SIC prediction results.

This study simultaneously predicts SIC, t2m, and SST through a multitask Transformer model, and the predicted t2m and SST are converted into a gate intensity map to correct the bias of SIC. Through this, we interpreted how atmospheric and oceanic environmental factors affected the SIC prediction results. In addition, by comparing the prediction results of SIC and environmental factors under conditions such as specific seasons and regions, where prediction is relatively unstable, we quantified the variable-specific weights under those conditions.

The gate intensity map used for SIC bias correction can itself be used as an uncertainty map, and expresses, as a spatial distribution, regions that are difficult for the deep learning model to predict. In addition, by comparing the impacts of each environmental factor by lead time, the contributions of variables can be identified at long-term and short-term prediction time points.

How to cite: Kim, W., Chung, I., Lee, G., Choo, M., and Im, J.: Enhancing sea ice concentration prediction with multi-task learning and conditional residual refinement, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16558, https://doi.org/10.5194/egusphere-egu26-16558, 2026.

EGU26-18020 | ECS | Posters on site | CR6.1

Global-scale modelling of mountain glacier evolution since the last interglacial 

Sjur Barndon, Augusto C. Lima, David M. Chandler, Abe Theodorus Wiersma, Eline Sterre Rentier, Raúl Prats Prats, and Suzette G.A Flantua

For most glaciated areas, detailed mountain glacier evolution since the last interglacial is largely unknown. Due to limitations of traditional numerical modelling, previous studies have typically operated at a coarse spatial resolution, limited study area size, or focused on major climate events. Here we address these limitations by applying the Instructed Glacier Model (IGM), a deep-learning ice-flow emulator enabling efficient GPU-accelerated transient simulations. We model mountain glacier evolution since 130 ka and up to the present-day at 500 m resolution across eight broad mountain ranges in North America, South America, Eurasia, and Africa. Paleoclimate variables are approximated and regionalised using a combination of global and regional climate proxy datasets. We perform 617 parameter-calibration experiments varying paleoclimate and ice-dynamic parameters, with an average runtime of 21 hours per experiment. Model performance is assessed using combined areal and volumetric validation at two known glacial states; the last glacial maximum and the present-day. We also introduce a reproducible probabilistic model-evaluation framework combining confusion matrix validation score and simulation rank to identify sets of acceptable model parameters rather than a single best-fit solution. Our results show that IGM can model realistic ice-flow patterns, glacier geometries, and transient evolution across full glacial-interglacial cycles, demonstrating that machine-learning models of ice dynamics generalise to new domains and conditions, although performance can decline at coarser spatial resolutions. Together, these results demonstrate the feasibility of global-scale, high-resolution, transient glacier modelling over orbital timescales using a deep learning instructed model, while providing a 100-year interval dataset including glacier extent, ice thickness, and ice flow patterns for the last glacial cycle.  

How to cite: Barndon, S., Lima, A. C., Chandler, D. M., Wiersma, A. T., Rentier, E. S., Prats, R. P., and Flantua, S. G. A.: Global-scale modelling of mountain glacier evolution since the last interglacial, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18020, https://doi.org/10.5194/egusphere-egu26-18020, 2026.

EGU26-18070 | ECS | Posters on site | CR6.1

Exploring Geo Foundation Models for Glacier Mapping Using Remote Sensing Data 

Farzaneh Barzegar, Norbert Kuehtreiber, and Silvia L. Ullo

Geo foundation models (GFMs) have recently emerged as a new paradigm in Earth observation (EO). They provide a promising approach for enhancing remote sensing analysis. GFMs enable faster and more generalised applications. They are deep learning models trained on large unlabelled datasets to learn general spatial, spectral, and contextual representations of the Earth’s surface. The datasets used are usually diverse in location, seasons, and even sensors. This diversity ensures that the model learns features that are as general as possible. This is vital because labelled data in remote sensing are limited, while high-quality unlabelled data are widely accessible. As a result, GFMs are increasingly viewed as a promising tool for scalable and robust environmental monitoring.

Among various EO tasks, glacier mapping is particularly relevant in the context of GFMs. Glaciers are located in hardly accessible regions, which makes ground-truth (GT) preparation difficult. Delineation of glaciers is often affected by seasonal snow and regional variability. Moreover, debris-covered and rock glaciers are harder to detect due to their complex landforms and their similarity to surrounding terrain. Accurate glacier delineation is crucial for monitoring cryospheric changes, assessing climate change impacts, managing water resources, and mitigating natural hazards.

In this study, we explore the applicability of GFMs for glacier mapping using multispectral Sentinel-2 imagery. We apply fine-tuning of pre-trained GFMs for glacier delineation, with the aim of assessing their potential in comparison with traditional deep learning approaches.

How to cite: Barzegar, F., Kuehtreiber, N., and L. Ullo, S.: Exploring Geo Foundation Models for Glacier Mapping Using Remote Sensing Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18070, https://doi.org/10.5194/egusphere-egu26-18070, 2026.

EGU26-19235 | ECS | Posters on site | CR6.1

Random forest predictions of tundra snow density elevate Arctic soil temperatures in CLM5.0 

Jonathan Rutherford, Nick Rutter, Leanne Wake, Georgina Woolley, Julia Boike, and Alex Cannon

Arctic snow exerts a critical control on winter soil temperature and carbon exchange, however representation of its properties in Earth System Models (ESMs) remains simplified. In the Community Land Model v5.0 (CLM5.0), recent updates to snow compaction schemes have led to overly dense tundra snow and excessive conductive heat loss, producing a persistent cold-soil bias. Here we developed a Random Forest (RF) regression model to derive tundra snow density from meteorological variables, trained on Arctic SVS2-Crocus (ASC) simulations supported by in-situ observations collected around peak annual SWE from Trail Valley Creek (TVC), Northwest Territories, Canada. The RF model reproduces ASC-simulated density evolution with a mean absolute error of 23 kg m-3 and an R2 of 0.90, matching field measurements more closely than CLM5.0. Future snow density predictions using the RF model driven by bias-corrected NA-CORDEX meteorology (2016 – 2100) indicate bulk snow densities 200 – 450 kg m-3 lower than CLM5.0 and more consistent with tundra conditions. Application of RF-derived snow densities decreases CLM5.0 winter season 10cm soil temperature RMSE by approximately 2 – 3 °C relative to field measurements (2017 – 2023) and increases future winter soil temperature projections (2016 – 2100) by 4 – 7 °C, highlighting the strong sensitivity of CLM5.0’s soil thermal regime to snow physical properties.

How to cite: Rutherford, J., Rutter, N., Wake, L., Woolley, G., Boike, J., and Cannon, A.: Random forest predictions of tundra snow density elevate Arctic soil temperatures in CLM5.0, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19235, https://doi.org/10.5194/egusphere-egu26-19235, 2026.

EGU26-20480 | ECS | Orals | CR6.1

Deep learning based spatio-temporal forecasting of snow cover in the Alps using remote sensing data  

Samip Narayan Shrestha, Andreas Dietz, Sarah Leibrock, and Claudia Kuenzer

Snow cover is a critical component of the earth’s climate and weather system, which exhibits high spatial and temporal variability. Therefore, we predict daily snow cover using spatio-temporal forecasting. Unlike traditional forecasting approaches, that require spatial or temporal aggregation, our approach employs deep learning models specifically designed for spatio-temporal data.  Spatio-temporal predictive learning has primarily focused on nowcasting and sub-seasonal forecasts at a daily scale with a lead time up to 15 days. However, we implemented the capability of using such models with long multi-year satellite image time series to predict at a daily scale annually, specifically for daily snow cover. In our research, we use the historical snow cover data from the DLR Global SnowPack remote sensing product, which is a daily cloud free 500m snow cover representation on the ground. We generate high resolution daily snow cover forecasts for up to 365 days (one year ahead) beginning from 1st July. We implemented models such as Convolutional Long Short-Term Memory (ConvLSTM) networks, convolutional encoder decoder architectures with attention mechanisms, and Vision Transformer (ViT) based models and adapted them for our use case. To further enhance our predictions, we also made adaptations to the models to include multivariate spatial and temporal data which are key drivers of snow cover variability into the model. Topographical feature maps derived from elevation, and time series of climatological indices (atmospheric oscillation patterns) are two examples. Validation against reference data demonstrates exceptional accuracy and F1-scores exceeding 84% across forecasts.

How to cite: Shrestha, S. N., Dietz, A., Leibrock, S., and Kuenzer, C.: Deep learning based spatio-temporal forecasting of snow cover in the Alps using remote sensing data , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20480, https://doi.org/10.5194/egusphere-egu26-20480, 2026.

EGU26-20684 | Posters on site | CR6.1

A deep learning-based emulator of the regional atmospheric model MAR for estimation of the Antarctic surface mass balance 

Achille Gellens, Cécile Agosta, Mikel N. Legasa, Mathieu Vrac, Charles Amory, and Christoph Kittel

Faithful modeling of Antarctic climate relies on capturing polar-specific processes at high spatial resolution (~10-30 km). Most CMIP earth system models (ESMs) used for climate projections inadequately represent physical processes that are key drivers in polar climates, and operate at resolutions too coarse to resolve them. Polar-oriented regional climate models (RCMs) are considered the state-of-the-art in modeling the atmosphere at high latitudes, where air-snow interactions are critical, but they are costly to run. This limits their use for exploration of large ensembles and scenarios as well as their potential of integrating into a coupled modeling pipeline.

In order to address these limitations, we develop an affordable surrogate model, or emulator, of the polar-oriented Modèle Atmosphérique Régional (MAR), using deep learning and a variant of the commonly used U-Net convolutional neural network architecture. The emulator is trained to predict 35 km-resolution daily maps of surface mass balance (SMB) components—snowfall, rainfall, run-off and sublimation—over the Antarctic ice sheet from large-scale atmospheric fields of ESMs, effectively learning the downscaling function embedded in MAR. To achieve this, we use a dataset composed of MAR simulations forced by 4 CMIP ESMs over the 1980–2100 period, covering SSPs 1-2.6, 2-4.5 and 5-8.5. We conduct different experiments to assess its best-case performance as well as its transferability to unseen scenarios and ESMs.

The emulator demonstrates strong in-domain skill, displaying high fidelity in reproducing both day-to-day and spatial synoptic variability of the predicted quantities. Long-term SMB trends and interannual variability through 2100 are also well-replicated, with predicted integrated surface mass change over the 1980–2100 period differing by only 1% from MAR. We find that the emulator is robust against unseen emission scenarios, with marginal increase of up to few percent in RMSE. Transferability to other ESMs proves more challenging but results remain promising.

The MAR emulator can be used to generate SMB forcings for ice-sheet models at a negligible computational cost compared to RCMs, allowing century-scale simulations to be produced within minutes and thereby enabling the exploration of a wide range of scenarios and ensemble members. We suggest the general framework of this work could allow for the emulation of MAR in any application where it can be traditionally used. Ongoing work is also investigating the applicability of the emulator within an atmosphere–ice sheet coupled framework.

How to cite: Gellens, A., Agosta, C., N. Legasa, M., Vrac, M., Amory, C., and Kittel, C.: A deep learning-based emulator of the regional atmospheric model MAR for estimation of the Antarctic surface mass balance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20684, https://doi.org/10.5194/egusphere-egu26-20684, 2026.

EGU26-22268 | Posters on site | CR6.1

Bayesian Optimisation for Antarctic Survey Planning 

Kim Bente, Roman Marchant, and Fabio Ramos

Remoteness, harsh environmental conditions, short field seasons, and high operational costs severely constrain the ability to collect observations of the polar cryosphere at scale. These limitations make efficient survey planning an important methodological need: data acquisition strategies must prioritise measurement locations that simultaneously (i) reduce model uncertainty and (ii) maximise scientific utility, for example by tightening constraints on projected ice sheet contributions to sea level rise. We address this need with Bayesian optimisation (BO), a probabilistic machine learning framework for black-box optimisation that uses a Gaussian process surrogate to model the target geospatial field and an acquisition function to formalise the trade-off between uncertainty reduction and scientific utility when proposing subsequent measurement locations. To showcase the approach, we consider a case study on planning airborne geophysical surveys of Antarctic ice thickness and bed topography, for which we introduce a set of novel acquisition functions tailored to Antarctic ice dynamics that translate cryospheric objectives into the BO framework:

  • The FluxUCB (Flux Upper Confidence Bound) acquisition function incorporates satellite-derived ice velocity observations to prioritise sampling uncertain, potentially high-flux regions under the current posterior, since such regions can exert a disproportionate influence on ice discharge.
  • Alternatively, PBBS (Probability of Bed Below Sea level) prioritises locations with a high posterior probability of marine-based grounding, thereby focusing effort on areas most relevant to assessing marine ice sheet instability (MISI).

In simulation, these objectives reduce posterior uncertainty per flight hour more efficiently than baseline strategies and more consistently target scientifically consequential regions. Together, these acquisition functions illustrate how BO can translate scientific priorities into an uncertainty-aware decision framework for data-efficient polar observation campaigns. More broadly, the framework has strong potential to extract greater value from limited polar field resources beyond airborne surveys, from optimising seismic survey design to informing ice core drilling site selection.

How to cite: Bente, K., Marchant, R., and Ramos, F.: Bayesian Optimisation for Antarctic Survey Planning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22268, https://doi.org/10.5194/egusphere-egu26-22268, 2026.

EGU26-1013 | PICO | CR6.2

Characterizing inter- and subglacial properties of a 3700 m plateau on the Grenzgletscher with active seismics 

Emma Chizzali, Joachim Wassermann, Coen Hofstede, and Elisa Mantelli

Located in the Monte Rosa massif in the Swiss Alps, the Grenzgletscher is one of the largest glaciers in the Alps, extending over approximately 2000 meters in height, with an accumulation zone that reaches up to 4500 meters and an ablation zone that descends to around 2500 meters. While its basal temperature reaches values of -13 °C at high elevations (Colle Gnifetti, 4450 m), it is temperate in the ablation zone, hence exhibiting at least one transition from frozen to temperate bed. As part of the ERC-funded project PHAST, a surface geophysics field campaign aimed at identifying the location of the frozen-to-temperate basal transition was conducted between 2024 and 2025. In this contribution we focus on the analysis of an active seismic survey conducted in 2024 to aid the characterization of basal conditions on a roughly 500 m x 500 m plateau at approximately 3700 m. The ELVIS-7 surface vibrator source was used to produce single-shot P-wave sweep signals along two lines of 48 geophones each, covering a total of 235 m, both parallel and perpendicular to the glacial flow. A velocity analysis was performed on the measured refracted waves, providing information on the upper part of the ice column and the depth of the firn layer. Deeper layers, the ice thickness, as well as the basal conditions, were studied via CMP/NMO processing and a phase-polarity analysis of the reflected waves. Finally, a post-stack migration was performed to obtain an accurate image of the glacier's subsurface along the receiver lines by accounting for possible steep-dipping interfaces or other structural complexities. In addition to revealing new information about the inter- and subglacial properties of the Grenzgletscher at high altitudes, the findings will be useful for identifying suitable drilling locations to study the physics of sliding onset in a natural laboratory, one of the main goals of PHAST.

How to cite: Chizzali, E., Wassermann, J., Hofstede, C., and Mantelli, E.: Characterizing inter- and subglacial properties of a 3700 m plateau on the Grenzgletscher with active seismics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1013, https://doi.org/10.5194/egusphere-egu26-1013, 2026.

EGU26-3139 | ECS | PICO | CR6.2

Influence of seasonally frozen soil properties on infiltration rates: based on field data 

Lisa Michaud, Michel Baraër, Christophe Kinnard, Annie Poulin, and Thomas Wespy

The presence of seasonal ground frost can markedly modify infiltration processes and runoff generation, yet its hydrological impacts remain inconsistently described. The literature alternately reports enhanced, uncertain, or negligible effects of frozen soils on runoff and infiltration. Few studies rely on direct field measurements of infiltration under frozen conditions, and none have directly linked infiltration rates to measured soil ice content. Expanding field observations across contrasting soil types is therefore necessary to better constrain winter hydrological behavior. Quantifying infiltration capacity under frozen conditions remains challenging, as soil freezing renders many standard measurement techniques ineffective. Yet such data are essential to understand the links between infiltration rates, soil ice content, and other frozen ground properties. We conducted field measurements using double-ring infiltrometers in a clayey agricultural field and a sandy clearing to quantify infiltration under both frozen and unfrozen conditions. A combination of in situ sensors and soil sampling was used to characterize soil ice and liquid water content, frost depth, and soil temperature. The resulting field observations reveal pronounced variability in infiltration rates under frozen conditions at both sites, with substantially greater variability in the clay-rich soil. Moreover, the relationships between infiltration rates and frozen soil properties—including frost depth, thermal state, and water and ice content—were found to depend strongly on soil composition.

How to cite: Michaud, L., Baraër, M., Kinnard, C., Poulin, A., and Wespy, T.: Influence of seasonally frozen soil properties on infiltration rates: based on field data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3139, https://doi.org/10.5194/egusphere-egu26-3139, 2026.

Antarctica, a critical regulator of global climate, faces threats to its permafrost and ecosystems from recent warming. However, a quantitative understanding of subsurface responses remains limited, hindering accurate environmental modeling. This gap hinders accurate modeling of future environmental changes. This study investigates the influence of rising air temperatures on active layer and permafrost characteristics... by quantifying the links between surface environmental changes and subsurface responses. From 2018–2024, we integrated meteorological observations, drone and satellite remote sensing, and geophysical surveys—electrical resistivity tomography (ERT) and ground-penetrating radar (GPR)—to assess atmosphere, surface, and subsurface changes. Our results indicated that the average annual temperature increased by ~1°C, extending the thaw season by ~50 days. Earlier snowmelt reduced albedo, increasing soil heat absorption and meltwater infiltration. The active layer thickened from 1.1 m to 1.5 m (maximum) and from 0.65 m to 0.85 m (dry sites). ERT indicated reduced resistivity at ~1 m depth, reflecting permafrost ice melt, and localized meltwater pooling at ~3 m depth. NDVI data showed increased vegetation activity. Our study shows that even slight warming can drive linked physical and ecological shifts in Antarctica, with implications for global climate feedbacks. Quantitative evidence of active layer thickening and permafrost degradation provides critical baseline data for improving prediction models. Future research should use year-round, three-dimensional monitoring and modeling to capture spatial variability and meltwater dynamics more accurately.

How to cite: Kim, K., Lee, J., Ju, H., and Kim, W.-K.: Monitoring Climate-Change Effects on the Barton Peninsula, King George Island, Antarctica: Evidence of Accelerated Active Layer Thickening, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3238, https://doi.org/10.5194/egusphere-egu26-3238, 2026.

EGU26-3860 | ECS | PICO | CR6.2

Tidally-modulated icequakes reveal mechanisms governing rifting on Larsen C Ice Shelf, Antarctic Peninsula 

Aisling Dunn, Alex Brisbourne, Sarah Thompson, Glenn Jones, J. Michael Kendall, Bernd Kulessa, Adrian Luckman, Katie E. Miles, and Bryn Hubbard

Suture zones, formed in the wake of peninsulas, are known to stall rifts on the Larsen C Ice Shelf, stabilising the shelf by delaying mass calving events. What exactly these rifts are composed of, and therefore how they are able to stall rifts, has remained elusive. Here we present direct evidence for brittle deformation within a suture zone immediately ahead of a detained rift tip, as recorded by a dense array of 29 low-noise accelerometers and three geophones. 251 icequakes were identified to originate within the network, 108 of which were successfully relocated to show a concentration of seismicity within the suture zone’s interior ice. No events were observed in the lowermost 20 m of the shelf, indicative of a porous basal marine ice layer or crevasse/cavity. The magnitude-frequency distribution yielded a catalogue b-value = 1.20 ± 0.11. For events from which source mechanisms could be derived, there is a correlation between rising/falling tides and explosive/implosive events, respectively. Collectively, these results are indicative of tidally-driven infiltration of seawater into the suture through the rift tip which will act to corrode the suture and promote brittle failure. The time-integrated effect of this process as the rift advects downstream will eventually weaken the suture zone sufficiently to allow for the rift to propagate despite lower downstream stresses, limiting the stabilising role of sutures towards the calving front.

How to cite: Dunn, A., Brisbourne, A., Thompson, S., Jones, G., Kendall, J. M., Kulessa, B., Luckman, A., Miles, K. E., and Hubbard, B.: Tidally-modulated icequakes reveal mechanisms governing rifting on Larsen C Ice Shelf, Antarctic Peninsula, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3860, https://doi.org/10.5194/egusphere-egu26-3860, 2026.

EGU26-4340 | PICO | CR6.2

Microstructural Characterization of Arctic Permafrost and Sea Ice From the Microscale to the Nanoscale Using X-Ray Microscopy 

Ross Lieblappen, Michelle Sama, Elizabeth Goodell, Dominic Mazzilli, Caleb Tilton, Ayden LaPoint, Geo Cuciti, Ben Boggio, Charles Schwenker, Olivia Rutkowski, Jill Nichols, and Andrew Vermilyea

Understanding the evolving state of the Arctic's upper permafrost and sea ice is crucial for tracking environmental effects, yet little is known about the nanostructure and distribution of microbial life within these environments. Recent advances in X-ray computed tomography technology have made it possible to image environmental samples not only at micron-scale resolution, but also at the nanoscale. Here we present high resolution images of permafrost and sea ice samples collected from Alaska, Nunavut, and Greenland. We have developed advanced segmentation techniques to characterize the microstructure, tracking variables such as porosity with depth. We have also developed techniques to use osmium staining to image microbes in situ within these samples at the nanoscale. At this resolution, we seek to connect physical and biological attributes of terrain state to improve our understanding of microbial distributions and microbially-mediated processes in cold regions.

How to cite: Lieblappen, R., Sama, M., Goodell, E., Mazzilli, D., Tilton, C., LaPoint, A., Cuciti, G., Boggio, B., Schwenker, C., Rutkowski, O., Nichols, J., and Vermilyea, A.: Microstructural Characterization of Arctic Permafrost and Sea Ice From the Microscale to the Nanoscale Using X-Ray Microscopy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4340, https://doi.org/10.5194/egusphere-egu26-4340, 2026.

EGU26-5188 | PICO | CR6.2

The induced polarization geophysical method applied to permafrost at various scales and for various frozen environments 

Andre Revil, Pierre-Allain Duvillard, Jessy Richard, Feras Abdulsamad, Florence Magnin, Clément Casotti, and Ahmad Ghorbani

The Dynamic Stern Layer (DSL) model is a reliable petrophysical model to comprehend induced polarization data at various scales from the representative elementary volume of a porous rock to the interpretation of field data at the cm to 100 m scales. We first review the DSL model in presence of ice and discuss the role of ice as an interfacial protonic dirty semi-conductor in the complex conductivity spectra of rocks and sediments. The electrical current polarizes the surface of the ice crystals and generates a very high chargeability that can reach one depending on the value of the volumetric content of ice. We apply the petrophysical model to a new set of complex conductivity spectra obtained in the frequency range 10 mHz-45 kHz using a collection of 25 rock samples including metamorphic and sedimentary rocks in the temperature range +15/+20°C to -10/-15°C. We observe that the model explains very well the observed data. We also investigate the role of porosity, cation exchange capacity, and freezing curve parameters on the complex conductivity spectra of crystalline and non-crystalline rocks during freezing. Laboratory experiments demonstrate that in most field conditions including permafrost conditions, surface conductivity associated with conduction on the surface of clay minerals (and alumino-silicates in general) is expected to dominate the overall conductivity response. Therefore Archie’s law cannot be used as a conductivity equation in this context because of the contribution of surface conductivity and has been strongly abused in the context of the applications of geoelectrical methods in the realm of the cryosphere. Time-domain induced polarization data obtained in field conditions are interpreted thanks to this updated DSL model. We selected three different test sites in order to apply the DSL model to very different conditions of low and high ice contents. A first survey is performed along a cross-section of a ridge in the Kangerlussuaq mountains of Greenland. We also performed a field survey close to Col des Vés (2846 m a.s.l., Tignes, French Alps, Site II). This site corresponds to a complex ground ice body overlying a substratum made of a low-porosity marble, both having high resistivity values. The front of this body is characterized by a small amount of residual ice while the roots are ice-rich. Therefore the porosity at this site is high and the ice content highly variable. This case study showcases the role of ice in the induced polarization data in terms of high chargeability values (close to 1 as predicted by the theory) at the roots of the complex ground ice body. A third site (Site III) corresponds to a profile crossing the Aiguille du Midi (3842 m a.s.l., Chamonix), also in the French Alps in a low porosity granitic environment. We end up with an application to a rock glacier (Site IV) to show how we can image the ice content. 

How to cite: Revil, A., Duvillard, P.-A., Richard, J., Abdulsamad, F., Magnin, F., Casotti, C., and Ghorbani, A.: The induced polarization geophysical method applied to permafrost at various scales and for various frozen environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5188, https://doi.org/10.5194/egusphere-egu26-5188, 2026.

EGU26-5686 | PICO | CR6.2

How do englacial radar features appear? Variability of horizons and facies in GPR data of Swiss glaciers 

Ilaria Santin, Christophe Ogier, Raphael Moser, Hansruedi Maurer, Huw Horgan, and Daniel Farinotti

Ground-penetrating radar (GPR) has long been a core tool for glacier investigations, and decades of surveys have created substantial archives of radar observations across a wide range of glaciers. Increasingly, attention is shifting from extracting ice thickness alone to exploiting a broader set of radar signatures (e.g. internal horizons, electromagnetic appearance such as transparent or scattering-dominated regions, and spatial variability) that may contain information on englacial structures. Realizing this potential requires understanding how such signatures manifest in real data, how variable their appearance can be across sites, and what this implies for interpretation confidence.

Here we investigate the variability of englacial GPR features using an archive of airborne and ground-based surveys on Swiss glaciers acquired by the Glaciology and Geophysics Groups at ETH Zurich between 2017 and 2024. The archive spans radar frequencies from 25 to 250 MHz and covers glaciers with contrasting geometries, dynamics, and site histories. To enable consistent description across heterogeneous datasets, we apply an observation-driven, appearance-based organization, informed by radar-facies concepts, classifying features by reflector geometry, continuity and coherence, as well as texture. We describe basal responses, internal layering, channelized features, transparent facies, and scattering-dominated facies, and illustrate each with representative examples from across the archive.

The examples show substantial variability and ambiguity in several features. Basal responses may be discontinuous, split into multiple reflections, obscured beneath scattering-dominated facies, or expressed as gradual facies transitions rather than discrete horizons. Similarly, internal layering varies in coherence, geometry, and continuity. Scattering-dominated facies show pronounced diversity in texture and organization. While it is often interpreted in relation to temperate ice, scattering is an electromagnetic response that is not diagnostic on its own of thermal regime, and a confident thermal interpretation requires independent constraints (e.g. borehole temperatures).

By presenting real-data examples of how radar signatures depart from commonly assumed expressions, we aim to increase awareness of the variability and interpretational ambiguity of englacial GPR features. By doing so, we highlight implications for interpretation confidence and future process-oriented studies supported by complementary observations.

How to cite: Santin, I., Ogier, C., Moser, R., Maurer, H., Horgan, H., and Farinotti, D.: How do englacial radar features appear? Variability of horizons and facies in GPR data of Swiss glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5686, https://doi.org/10.5194/egusphere-egu26-5686, 2026.

EGU26-5821 | PICO | CR6.2

GNSS measurement of seasonal ice flow velocity of the northeast Greenland ice stream and Jakobshavn Isbræ, Greenland. 

Shfaqat Abbas Khan, Javed Hassan, William Colgan, Kuba Oniszk, Gong Cheng, Alicia Bråtner, Mathieu Morlighem, Sina Marie Felten, Helene Seroussi, Christian Solgaard, Danjal Berg, Valentina Barletta, Anja Løkkegaard, Dominik Fahrner, Anuar Togaibekov, and Tobias Socher

In 2016, we established the first network of GNSS stations on the Northeast Greenland Ice Stream (NEGIS), enabling continuous monitoring of ice flow motion and surface elevation changes. These stations have revealed both short-term variability and longer-term accelerations that propagate far inland from the terminus (Khan 2022; Khan 2024), highlighting the dynamic coupling between the glacier front and the interior of the ice sheet. Building on this effort, in 2024 we deployed four additional GNSS stations on Jakobshavn Isbræ, one of Greenland’s fastest-flowing outlet glaciers. All stations on both Jakobshavn and NEGIS are located along the main glacier trunks, spanning distances of ~20 to ~200 km from the terminus, thereby capturing spatial gradients in flow and deformation.

The GNSS sites also enable direct validation of satellite-derived surface elevation products (ICESat-2 and CryoSat-2). Whereas satellite altimetry provides repeat measurements of ice-surface elevation once per month, GNSS observations deliver continuous, hourly records of both vertical and horizontal ice motion. This high temporal resolution allows us to resolve short-lived dynamic events, seasonal signals, and longer-term trends that are not detectable from spaceborne sensors alone. Together, these complementary datasets provide powerful constraints for improving ice-flow models and for assessing the future evolution and stability of the Greenland Ice Sheet.

In addition, we apply GNSS interferometric reflectometry (GNSS-IR) to the ice-sheet environment, using reflected GNSS signals to infer changes in ice-surface height and physical properties such as roughness and snow accumulation. This technique adds a new observational dimension to the GNSS network, further enhancing its value for characterizing glacier–atmosphere interactions and surface processes.

How to cite: Khan, S. A., Hassan, J., Colgan, W., Oniszk, K., Cheng, G., Bråtner, A., Morlighem, M., Felten, S. M., Seroussi, H., Solgaard, C., Berg, D., Barletta, V., Løkkegaard, A., Fahrner, D., Togaibekov, A., and Socher, T.: GNSS measurement of seasonal ice flow velocity of the northeast Greenland ice stream and Jakobshavn Isbræ, Greenland., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5821, https://doi.org/10.5194/egusphere-egu26-5821, 2026.

EGU26-6145 | ECS | PICO | CR6.2

Acoustic monitoring of proglacial discharge at Qaanaaq Glacier, Northwest Greenland 

Tomohiro Nakayama, Evgeny Podolskiy, Takuro Imazu, Kotaro Yazawa, and Shin Sugiyama

Glaciers around the world have experienced substantial mass loss due to global warming (Hugonnet et al., 2021). In Greenland, meltwater runoff is one of the major contributors to mass loss from the Greenland Ice Sheet and surrounding glaciers (Mouginot et al., 2019). This meltwater increases the discharge of proglacial rivers and poses a growing flood hazard to local communities (Kondo et al., 2021). Therefore, there is an urgent need to develop passive, robust, and low-maintenance methods for monitoring proglacial discharge under rapidly changing channel conditions.

Recent studies have shown a strong correlation between proglacial river discharge and fluvial sound (Podolskiy et al., 2023). Fluvial sound is mainly generated by air-bubble entrainment and collapse within turbulent flow features such as rapids and waterfalls, and its amplitude and spectral characteristics systematically respond to changes in discharge (Bolghasi et al., 2017). Passive acoustic monitoring therefore enables non-invasive and cost-effective discharge observation by simply recording the self-generated sound of a river, yet its applicability and limitations remain insufficiently understood.

In this study, we investigate the potential of passive acoustic monitoring to track proglacial discharge at Qaanaaq Glacier in northwestern Greenland (77°28’ N, 69°14’ W). During the summer of 2024, we deployed four passive acoustic sensors along the proglacial river and continuously recorded fluvial sound. Acoustic power in the 94–375 Hz frequency band showed a strong correlation with river discharge (R ≈ 0.90). Cross-correlation analysis between two sensors separated by 1,850 m revealed highly correlated acoustic signals (R = 0.90) with repeatable time lags of up to approximately one hour, although data gaps occurred during very low- and high-discharge conditions when the acoustic time lag became poorly resolved. This limitation suggests that larger sensor separations or array-based deployments may be required to robustly resolve time lags under variable flow conditions.

In addition to fluvial sound, the acoustic sensors recorded traffic-related noise from a bridge crossing the river. More than 200 traffic events were detected, providing supplementary information relevant to local flood risk and infrastructure usage. The usage of bridge reached maximum around 13 to 16 local time of Qaanaaq (LT), whereas discharge reached maximum around 18 to 23 LT. The peak in bridge usage occurred during the rising phase of discharge, highlighting the importance of early-stage flood awareness for local communities.

These results demonstrate that passive acoustic monitoring offers a low-cost, non-invasive tool that can complement conventional methods for monitoring proglacial river discharge, particularly in dynamically evolving glacial river systems. In addition, acoustic observations can provide complementary information on human activity near rivers, which is relevant for local flood-risk awareness and infrastructure management.

How to cite: Nakayama, T., Podolskiy, E., Imazu, T., Yazawa, K., and Sugiyama, S.: Acoustic monitoring of proglacial discharge at Qaanaaq Glacier, Northwest Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6145, https://doi.org/10.5194/egusphere-egu26-6145, 2026.

EGU26-6792 | ECS | PICO | CR6.2

Estimation of Liquid Water Content and Density in the Surface Layer of the Snowpack from the Phase and Amplitude of SFCW Radar Signals 

Adrián Subías Martín, Iñigo Salinas, Víctor Herráiz-López, Samuel T.Buisán, and Rafael Alonso

The precise determination of liquid water content (LWC) and density in the surface layer of the snowpack is crucial for understanding hydrological, energetic, and mechanical processes in snow-covered environments. The surface quality of the snowpack controls energy exchanges with the atmosphere and influences the electromagnetic response of the medium. However, the simultaneous and non-intrusive estimation of density and LWC remains challenging due to the strong interdependence between these parameters and the limited ability of many methods to separate them.

This work presents a method for the simultaneous estimation of density and liquid water content in the surface layer of a snowpack using a Stepped Frequency Continuous Wave (SFCW) radar operating in the 0.6–6 GHz range. The methodology is based on identifying, within the Fourier transform of the received signal, the peak corresponding to the air–snow interface. From this peak, two fundamental quantities are extracted (amplitude and phase) which are used to estimate the electromagnetic and physical properties of the snowpack surface.

Phase differences of the reflection peak are used to estimate LWC, as liquid water is the only constituent of the snowpack that introduces a significant imaginary component to the refractive index within the considered frequency range. In this interval, the complex permittivity of water exhibits high values, with a dominant effective imaginary part, while air introduces no losses and ice has an imaginary component at least three orders of magnitude smaller than that of water. Consequently, the accumulated phase shift of the reflected signal is directly controlled by the presence of liquid water, allowing small variations in LWC to be detected in the phase of the reflection peak.

The amplitude of the reflection peak depends on the total material content at the surface, as all constituents contribute to the real part of the effective refractive index. The amplitude is influenced by both snow density and LWC. Since the liquid water fraction is obtained beforehand from the phase, the relative proportions of air and ice can be estimated. From this information, the dry snow density is calculated, and through a volumetric balance, the total density of the surface layer and the LWC are determined.

The method is supported by preliminary calculations of the reflection coefficient Γ, which are used to derive calibration relationships for both phase and amplitude. Validation is carried out using synthetic snow structures representative of different surface conditions, including variations in dry snow density, liquid water content and layer thickness. In addition, initial field experiments have been conducted, showing responses consistent with the synthetic analysis and demonstrating the applicability of the approach under realistic conditions.

The results indicate that the combination of phase and amplitude constitutes a robust, non-intrusive tool for in situ monitoring of the snowpack, with the potential to detect early-stage compaction, melting, refreezing and rainfall events on snow.

How to cite: Subías Martín, A., Salinas, I., Herráiz-López, V., T.Buisán, S., and Alonso, R.: Estimation of Liquid Water Content and Density in the Surface Layer of the Snowpack from the Phase and Amplitude of SFCW Radar Signals, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6792, https://doi.org/10.5194/egusphere-egu26-6792, 2026.

EGU26-7859 | ECS | PICO | CR6.2

A permittivity sensor integrated into melting probes for in-situ cryospheric characterisation 

Fabian Becker, Jan Audehm, Georg Böck, Mia Giang Do, Enrico Ellinger, Marco Feldmann, Gero Francke, Niklas Haberberger, Klaus Helbing, Lukas Rechenberg, Martin Vossiek, and Christopher Wiebusch

The TRIPLE project aims to develop key technologies for a future space mission dedicated to the search for extraterrestrial life on Jupiter’s moon Europa. The mission concept is based on a melting probe designed to penetrate Europa’s ice shell and deploy scientific instruments into the underlying subsurface ocean to search for life and biosignatures. To validate the feasibility of this approach, the developed technologies are tested stepwise in terrestrial analogue environments under extreme conditions.

Within the TRIPLE-FRS project, a Forefield Reconnaissance System (FRS) for these ice-penetrating melting probes is being developed that combines radar and sonar sensing to scan the probe’s forefield. To enable in-situ correction of radar and sonar wave velocities, an additional sensor is integrated into the melting probe to measure the complex permittivity of the surrounding medium.

This contribution presents the integration of the permittivity sensor into the melting probe TRIPLE-IceCraft, the achievable measurement accuracy for a wide range of dielectrics, and the results of validation experiments conducted in controlled freezer environments and on alpine glaciers. Furthermore, the role of the sensor system within an upcoming Antarctic field campaign at Neumayer Station III during the 2026/2027 season is outlined.

How to cite: Becker, F., Audehm, J., Böck, G., Do, M. G., Ellinger, E., Feldmann, M., Francke, G., Haberberger, N., Helbing, K., Rechenberg, L., Vossiek, M., and Wiebusch, C.: A permittivity sensor integrated into melting probes for in-situ cryospheric characterisation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7859, https://doi.org/10.5194/egusphere-egu26-7859, 2026.

EGU26-8251 | ECS | PICO | CR6.2 | Highlight

Towards a New Regional Ice Thickness Dataset: UAV-Borne GPR for Quantifying Remaining Ice Volumes of Alpine Glaciers 

Anna Siebenbrunner, Markus Keuschnig, and Michael Krautblatter

Geophysical investigations of Alpine glaciers are essential for quantifying ice thickness and internal structures, yet traditional ground-based Ground-Penetrating Radar (GPR) remains logistically constrained in complex, high-altitude terrain. The emergence of Unoccupied Aerial Vehicle (UAV) platforms provides a transformative opportunity for radioglaciology, allowing for rapid, high-resolution data acquisition. While conventional mass balance methods focus on annual or subseasonal superficial mass changes, GPR enables the determination of the total remaining ice volume – a prerequisite for accurately forecasting future glacier evolution and glacial runoff. However, traditional ground-based GPR surveys are often logistically demanding and hazardous due to crevasses and unstable terrain, which frequently limit the spatial density and resolution of the resulting datasets. Recent advances in UAV technology have enabled the integration of lightweight geophysical sensors, offering a safer and more efficient alternative that significantly enhances spatial coverage and data resolution in glaciated environments.

This contribution presents results from ten glaciers in the Eastern Alps surveyed in 2024 and 2025 using a UAV-borne GPR system. The investigated sites range in size from 0.09 km² to 2.15 km² and encompass a diverse range of morphological types, including debris-covered, plateau, and valley glaciers. Furthermore, the study areas span contrasting geological settings and include both glaciers affected by anthropogenic activities (e.g., ski resort infrastructure) and largely undisturbed systems. Based on two years of UAV-based data acquisition, we provide a critical assessment of the associated methodological challenges, data quality limitations, and logistical constraints. We highlight key lessons learned regarding the performance of the UAV-borne GPR system in diverse cryospheric settings and outline future developments aimed at expanding this dataset to improve regional glacier volume estimates. Finally, we invite fellow researchers working with UAV-borne GPR to collaborate on establishing a new glacier thickness database.

How to cite: Siebenbrunner, A., Keuschnig, M., and Krautblatter, M.: Towards a New Regional Ice Thickness Dataset: UAV-Borne GPR for Quantifying Remaining Ice Volumes of Alpine Glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8251, https://doi.org/10.5194/egusphere-egu26-8251, 2026.

Electromagnetic induction (EM) is one of the established techniques for in-situ sea ice thickness measurement. It is typically implemented using shipborne or airborne transmitter-receiver coil systems (e.g., EM 31, AWI, DIGHEM) operating at single or multiple frequencies. While this method can acquire reliable sea ice thickness data, limitations exist in case of thin ice and regions with severely variable ice thickness . The fixed coil spacing (e.g., 3.66 m for EM 31) constrains detection sensitivity for thin ice, particularly in shipborne or airborne measurements where altitude variations can significantly affect inversion accuracy . To enhance thin-ice detection capability and inversion stability, this study proposes a novel electromagnetic induction method utilizing dual receiver coils.

This method retains a single transmitter coil and incorporates two receiver coils with a spacing of 0.5 m. By increasing the amount of measured data, the response characteristics for thin-layer targets are optimized. Based on typical polar sea ice conductivity parameters (seawater ~2.6 S/m, sea ice ~0.06 S/m), electromagnetic numerical simulations were conducted for sea ice with thicknesses ranging from 1 to 5 m. These simulations analyzed the response relationship between the secondary field signal and ice thickness under the dual-receiver coil configuration. The results indicate that, compared to traditional single-receiver coil systems, data from the dual-receiver coils exhibit greater sensitivity to variations in thin ice thickness and help reduce inversion uncertainty caused by fluctuations in measurement altitude.

Building on the simulation data, this study further developed an inversion algorithm for dual-receiver coil data. This algorithm integrates dual-channel data continuously acquired along the same direction to achieve accurate and stable inversion of sea ice thickness. Preliminary verification shows that the inversion uncertainty of this method for thin ice in the 1~3 m range is significantly lower than that of conventional methods. This approach provides a new technical pathway for developing next-generation portable, low-platform (ground-based, shipborne, or UAV-borne) sea ice thickness detection equipment. It contributes to enhancing capabilities in climate research and safety assurance for polar navigation.

How to cite: Zou, C., Yuan, C., Peng, C., and Markov, A.: Sea Ice Thickness Measurement in Polar Environments: An Electromagnetic Detection Approach Using a Dual-Receiver Coil System, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8861, https://doi.org/10.5194/egusphere-egu26-8861, 2026.

EGU26-9490 | ECS | PICO | CR6.2

Validation of shared parameterisation for cosmic ray neutron sensors measuring snow water equivalent in the Italian Alps 

Mario Gallarate, Nicola Colombo, Enrico Gazzola, Mauro Valt, Christian Ronchi, Luca Lanteri, Roberto Dinale, Rudi Nadalet, Stefano Ferraris, Alessio Gentile, Davide Gisolo, Michele Freppaz, and Fiorella Acquaotta

Seasonal snow cover plays a fundamental role in sustaining human activities in mountain communities. Runoff originating  from the European Alps is a primary water source for millions of people. However, Alpine snow resources are increasingly threatened by rising temperatures and changes in precipitation patterns due to climate change. These factors underscore the need for accurate and widespread monitoring of the Alpine snow resources.

From a hydrological perspective, snow water equivalent (SWE) is crucial to assess the water amount stocked in the snowpack and, therefore, the water availability after snowmelt. The most historically widespread SWE measurement practices consist in the direct assessment of the snow bulk density through field campaigns involving vertical coring or snow pits. Although these methods are highly accurate, they provide limited temporal and spatial coverage due to the significant manpower required and the inaccessibility of many sites during the snow season.

In the last decades, the development of sensors based on cosmic ray neutron sensing (CRNS) allowed the measurement of continuous SWE data in already monitored sites, filling the gaps associated with manual measurements. However, applying CRNS to monitor snowpacks in inaccessible sites remains largely unexplored as the standard procedure to retrieve SWE from neutron counts relies on site-specific parameters derived from reference measurements.

This work presents a network of 26 CRNS sensors located across the Italian Alps. The network is among the most extensive of its kind both in terms of both the number of probes and elevation range (1422 – 2901 m a.s.l.). Its broad coverage provides unprecedented insights into the possibility of retrieving SWE data independently of most of the site-specific features usually required. Notably, the parameterisation used to convert neutron counts into SWE is common to all  probes in the network.

Manual SWE data from 13 sites within the network, collected during the 2023–2024 and 2024–2025 snow seasons, were used to calibrate and validate the network-wide parameterisation.  The calibration process involved 35 direct SWE measurements performed at 6 sites during the first half of the 2023 – 2024 season. A total of 111 manual SWE data were used as the validation dataset.

The analysis shows that the application of a shared set of parameters results in a good representation of the snowpack characteristics. Moreover, the data from unmonitored sites of the network show high correlations with monitored sites at similar elevations. These results suggest that deploying CRNS probes can be used to overcome common limitations of snow monitoring, such as site accessibility issues, lack of manpower to perform manual measurements, and safety hazards linked to the harsh mountain environment.

This abstract is part of the NODES project which has received funding from the MUR–M4C2 1.5 of PNRR funded by the European Union - NextGenerationEU (Grant agreement no. ECS00000036).

How to cite: Gallarate, M., Colombo, N., Gazzola, E., Valt, M., Ronchi, C., Lanteri, L., Dinale, R., Nadalet, R., Ferraris, S., Gentile, A., Gisolo, D., Freppaz, M., and Acquaotta, F.: Validation of shared parameterisation for cosmic ray neutron sensors measuring snow water equivalent in the Italian Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9490, https://doi.org/10.5194/egusphere-egu26-9490, 2026.

EGU26-9759 | ECS | PICO | CR6.2

Inferring the crystal orientation fabric of the Northeast Greenland Ice Stream using polarimetric radar data 

Niels F. Nymand, David A. Lilien, and Dorthe Dahl-Jensen

The crystal orientation fabric (COF) of glacial ice strongly influences its mechanical properties and evolves with flow. Large-scale ice flow models currently neglect COF evolution, but including it is becoming increasingly feasible. However, observations are still very sparse and often depth-averaged or point measurements. Radars, and especially polarimetric radars, are sensitive to the COF due to the birefringence of ice and provide a relatively easy way to collect observations that can be used to infer the anisotropy and orientation of the COF. In this study, we formulate the problem of inferring the COF from polarimetric radar data as an inverse problem to derive depth-resolved horizontal COF anisotropy. The method is applied to polarimetric radar data from the Northeast Greenland Ice Stream (NEGIS), where previous methods have struggled due to the high anisotropy. The method relies on an iterative linearization of the Fujita radio-wave depolarization matrix model to estimate COF orientation and scattering anisotropies. It also employs a linear maximum likelihood solution to derive eigenvalue differences from travel-time anisotropies. The inversions generally recreate the observed power anomalies and reveal a strong increase in horizontal anisotropy at shallow depths in NEGIS, followed by a rapid decrease near the ice stream base, likely due to recrystallization processes. The inversion also shows a near flow-aligned COF close to the onset of the ice stream, with increasing misalignment along a 30 km flowline downstream.

How to cite: Nymand, N. F., Lilien, D. A., and Dahl-Jensen, D.: Inferring the crystal orientation fabric of the Northeast Greenland Ice Stream using polarimetric radar data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9759, https://doi.org/10.5194/egusphere-egu26-9759, 2026.

EGU26-10833 | PICO | CR6.2

Hydrothermally influenced rock slope kinematics: The role of water on Wisse Schijen 

Samuel Weber, Marcia Phillips, Mauro Häusler, Robert Kenner, Raphael Moser, Sebastian Summermatter, Martin Volken, and Alex Bast

Long-term ground temperature records from high-alpine environments document a persistent warming trend and a progressive thickening of the active layer of permafrost across the European Alps. This thermal evolution directly affects the internal hydrological regime of rock slopes. In frozen rock masses with ice-filled fractures, hydraulic permeability is markedly reduced relative to unfrozen conditions. Permafrost warming and thawing thus promote water infiltration, perched water, and elevated water pressures once ice melt occurs. Surface water input infiltrates through fracture systems or heterogeneous ground layers within the active layer, causing local concentrations of convective heat transport that can initiate the development of preferential thaw pathways in the underlying permafrost.

Such hydrothermal interactions are expected to exert a first-order control on the stability and kinematics of failure-prone rock slopes. However, the role of water in governing thermo-mechanical coupling and deformation in mountain permafrost remains poorly understood. Evidence for the presence, distribution, and temporal variability of water in permafrost rock slopes is scarce, with only a few studies documenting temporal changes in water content using piezometric measurements. In-situ observations and laboratory experiments remain limited, providing only partial information on the role of water in frozen ground. Consequently, non-conductive heat fluxes, phase-change processes, and their implications for rock slope deformation are still insufficiently quantified, primarily due to their strongly nonlinear nature and the challenges associated with direct measurement.

To address the role of water in permafrost rock slope dynamics, we investigate the Wisse Schijen study site (Valais, Switzerland), a deep-seated permafrost rock slope instability with an estimated volume exceeding 1 million m³, located on an approximately 40° steep, east-facing slope between 3010 and 3140 m a.s.l. We apply a multi-method analysis that integrates spatially and temporally resolved geological, thermal, kinematic, and seismic data and relates these observations to atmospheric and hydrological forcing. The combined dataset reveals a clear kinematic response of the rock slope to hydrothermal forcing, manifested by seasonally variable deformation patterns that coincide with periods of enhanced water availability and elevated subsurface temperatures. Our results indicate that water-driven thaw processes and associated hydrogeological changes likely reduce effective stresses and alter the geotechnical properties of the rock mass, thereby modulating deformation rates and kinematic behavior. These observations highlight the critical role of hydrothermal processes in controlling the mechanical response of permafrost rock slopes and emphasize the importance of explicitly accounting for hydrothermal coupling in assessments of high-alpine slope stability under ongoing climate warming.

How to cite: Weber, S., Phillips, M., Häusler, M., Kenner, R., Moser, R., Summermatter, S., Volken, M., and Bast, A.: Hydrothermally influenced rock slope kinematics: The role of water on Wisse Schijen, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10833, https://doi.org/10.5194/egusphere-egu26-10833, 2026.

EGU26-12129 | PICO | CR6.2

The Frost.ini project: A framework enabling 4D electrical resistivity investigations on a rock glacier 

Antonio Bratus, Emanuele Forte, and Massimo Giorgi

The Frost.ini project, Permafrost degradation and instability of high-mountain infrastructures, funded within the Interreg VI-A Italy–Austria Programme 2021–2027, aims to develop a holistic analysis of permafrost in order to monitor its degradation and integrate risk mitigation measures into territorial management policies, thereby improving the resilience of high-altitude infrastructures.

The project is structured around a series of pilot actions carried out at sites selected according to strategic and scientific criteria, including the availability of previous studies.

The Casera Razzo rock glacier is located in the northern sector of the Friulian Dolomites, in northeastern Italy, within an alpine setting of significant geomorphological and geological interest. Traditionally classified as a relict landform based solely on surface morphology, it instead shows clear evidence of frozen material within its interior. Geophysical investigations and microclimatic measurements have identified interstitial ice and small ice lenses, indicating the presence of residual permafrost even during the period of maximum seasonal thaw.

The geoelectrical method, and in particular Electrical Resistivity Tomography (ERT), is a highly effective tool for the construction of geological models and for permafrost monitoring, as it allows non-invasive subsurface investigation and the repetition of measurements over time.

An initial resistivity model based on 2D data acquired in 2015 confirmed the presence of ice. The 3D survey carried out in 2025 using the FullWaver system by IRIS Instruments, partly overlapping the previous survey area, generated a three-dimensional resistivity model that quantified the ice volumes and provided important insights into the evolution of the rock glacier.

The results demonstrate that the FullWaver system is suitable for complex electrical investigations in environmentally challenging settings. By exploiting its capabilities, it is possible to obtain key information on permafrost evolution, which is essential for the modelling of future scenarios.

How to cite: Bratus, A., Forte, E., and Giorgi, M.: The Frost.ini project: A framework enabling 4D electrical resistivity investigations on a rock glacier, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12129, https://doi.org/10.5194/egusphere-egu26-12129, 2026.

EGU26-12321 | ECS | PICO | CR6.2

Gravity surveys for mountain permafrost quantification: the Sadole Rock Glacier (Italy) 

Ilaria Barone, Alessandro Ghirotto, Mirko Pavoni, Alberto Carrera, and Jacopo Boaga

Rock glaciers are permafrost landforms typical of high-altitude mountain environments, composed of varying proportions of ice, rock debris, air, and occasionally liquid water. Their internal structure is highly heterogeneous and evolves in response to climatic, hydrological, and geological forcing. Due to global warming, the investigation of mountain permafrost has become increasingly important for evaluating its stability, ice content, and hydrology. In this context, non-invasive geophysical techniques have proven to be effective tools for imaging subsurface conditions in periglacial environments.

The Sadole Rock glacier, located in the Eastern Italian Alps, has been extensively studied in the last years through several geophysical campaigns. In this study, we present the results of a complementary gravity investigation performed along two quasi-parallel profiles, with the aim of estimating the ice fraction in the permafrost and its spatial distribution. Data were collected between October 2024 and June 2025 using a relative gravimeter Scintrex CG-5 and were processed to finally obtain the complete Bouguer anomaly (BAC) along the profiles. BAC data show negative values, that we assume being related to the presence of ice. 2D forward modelling was carried out considering different scenarios. In all the cases examined, the bedrock depth was set based on preliminary geophysical information, while permafrost densities were varied as a function of the ice content considered.

The obtained results show the potential of gravity anomaly data for the estimation of the ice fraction of mountain permafrost. However, preliminary information is needed to constrain the density model (such as a resistivity model derived from ERT measurements), due to the high degree of non-uniqueness of the solution.

How to cite: Barone, I., Ghirotto, A., Pavoni, M., Carrera, A., and Boaga, J.: Gravity surveys for mountain permafrost quantification: the Sadole Rock Glacier (Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12321, https://doi.org/10.5194/egusphere-egu26-12321, 2026.

We present an application of ground-penetrating radar-based (GPR) common midpoint method (CMP) to quantify temporal changes in firn density and compaction rates, complemented by direct observations, such as firn cores at the accumulation area of the Grosser Aletschgletscher. We identify the last summer horizon and characterise the firn stratigraphy using firn core and isotope analysis. The comparison of the acquired firn core and the CMP-derived density-depth profile from the Ewigscheefeld shows similar density-depth variations. Our three CMP gather results illustrate the spatially varied depth to the pore close-off density (830 kg/m³), which is approximately 25 and 17 m at Ewigschneefeld and Jungfraufirn, respectively,  depicting the spatial variation in firn densification. Further, we identified 10-15 annual layers from the CMP-derived internal reflection horizons (IRHs) by comparing estimated snow water equivalent (SWE) with point mass-balance measurements. Temporal changes in firn density-depth profiles obtained from CMP data measured a year apart illustrate that certain identified annual layers at shallower depths are denser than deeper layers (100-150 kg/m³). Our results demonstrate that the influence of summer melts is a dominating process on Alpine firn densification, rather than the conventional densification driven by accumulated snow. We investigated the temporal changes in spatial firn stratigraphy from a 4.4 km long GPR profile by comparing it with a previously measured GPR transect from the same location. Our investigation exemplifies the possibility of quantifying firn densification and compaction rates using unique temporal GPR measurements in an Alpine glacier.

How to cite: Patil, A. and Mayer, C.: Investigating temporal changes in the Alpine firn density and compaction rate using repeat ground penetrating radar measurements at the accumulation areas of the Grosser Aletschgletscher, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12798, https://doi.org/10.5194/egusphere-egu26-12798, 2026.

EGU26-13345 | ECS | PICO | CR6.2

Laboratory and field validated temperature-resistivity relations in bedrock permafrost 

Maike Offer, Johannes Leinauer, Samuel Weber, Saskia Eppinger, Ingo Hartmeyer, and Michael Krautblatter

Electrical resistivity tomography (ERT) has become a well-established geophysical method for monitoring the thermal state of permafrost sites. However, quantitative interpretation of ERT data requires corresponding temperature information, either from direct borehole temperature measurements or from laboratory-based calibrations. Borehole measurements are costly to implement and remain scarce in alpine environments. Temperature-resistivity relations derived from laboratory experiments are generally site-specific, restricted to individual lithologies, and only rarely validated against field observations.

Here, we present temperature-resistivity relations derived from laboratory experiments on 12 low-porosity rock samples representing different sedimentary, metamorphic, and igneous lithologies. The samples were collected from permafrost-affected summit areas of Zugspitze (DE/AT), Großglockner (AT), Kitzsteinhorn (AT), Gemsstock (CH), Steintälli (CH), Gámanjunni-3 (NOR), Nordnes (NOR), and the Mannen plateau (NOR). The temperature-resistivity pathways are analysed with respect to porosity and mineral composition for unfrozen, frozen, and supercooled conditions. Particular emphasis is placed on the temperature range between -5 and +5 °C, where relevant mechanical changes occur, but also the major electrical transition due to the increasing partial freezing of pore water content.

The transferability of laboratory results to field observations is evaluated using a year-round automated ERT monitoring dataset from the Kitzsteinhorn (3.029 m a.s.l.), complemented by deep borehole temperature measurements along the profile. Deviations between field resistivity values and laboratory values can be explained by temporal and spatial effects. In the field, other than in the lab, seasonal pressurised water flow occurs in fractures, evidenced by piezometric measurements reaching peak values of 1.2 bar, and rock heterogeneities lead to enhanced drying and freezing of disintegrated rock blocks.

We anticipate that our provided temperature-resistivity pathways for different lithologies under unfrozen, frozen, and supercooled conditions will improve quantitative interpretation of ERT monitoring data and the assessment of permafrost warming and associated rock slope instabilities.

How to cite: Offer, M., Leinauer, J., Weber, S., Eppinger, S., Hartmeyer, I., and Krautblatter, M.: Laboratory and field validated temperature-resistivity relations in bedrock permafrost, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13345, https://doi.org/10.5194/egusphere-egu26-13345, 2026.

EGU26-17065 | PICO | CR6.2

Transient electromagnetic responses to deep low resistivity targets beneath thick resistive ice sheet 

Yuanyuan Zhang, Changchun Zou, Jacopo Boaga, and Cheng Peng

Thick, high-resistivity ice sheets extensively cover bedrock and sedimentary layers, posing significant challenges for the identification of subglacial hydrological systems and associated geological structures. Subglacial water systems not only play a crucial role in regulating ice-sheet dynamics and material transport, but also serve as important indicators of deep geological environments, fluid activity, and potential mineralization conditions.However, high-resistivity ice sheets significantly enhance electromagnetic energy attenuation during field propagation, resulting in insufficient recoverable low-frequency signals and thereby limiting the detectability of deep low-resistivity anomalies. This challenge is widespread in polar environments and exhibits strong similarities to those encountered in other high-resistivity-covered mineral exploration settings.

In this background, this study applies the loop-source transient electromagnetic (TEM) method to to systematically analyze the spatial distribution characteristics of transient attenuation curves and electric field components by constructing various underground models (e.g., subglacial water systems and fluid-rich anomalies). Results indicate:

(1) In models containing high-conductivity anomalies (such as saturated sedimentary layer), the presence of conductive bodies significantly slows electromagnetic field diffusion. As a result, response signals maintain relatively high amplitudes during late-time sampling, resulting in attenuation curves exhibiting a characteristic S-shaped bulge. This indicates that transient electromagnetic methods possess high discrimination capability for identifying water-bearing low-resistivity anomalies.

(2) As the ice thickness increases from 50 m to 500 m, the transient electromagnetic response curve exhibits an overall rightward and downward shift. The rightward shift reflects the elongated propagation paths and delayed response times of electromagnetic fields within thick resistive cover, whereas the downward shift indicates enhanced attenuation of electromagnetic signals by the overburden, thereby reducing sensitivity to deep subsurface structures. In addition, increasing cover thickness amplifies response differences among distinct subsurface targets, leading to reduced resolution in inverted models.

(3) Under conditions of thin ice cover, differences in transient responses induced by varying transmitter loop sizes are relatively minor. However, as ice thickness increases, the required transmitter magnetic moment rises substantially. Large transmitter loops (e.g., 300 m and 500 m) generate stronger transient electromagnetic fields owing to their higher magnetic moments. Their late-time responses exhibit higher amplitudes and longer persistence, indicating enhanced sensitivity to deep low-resistivity anomalies. This improvement contributes to better imaging performance and more reliable identification of deep subsurface targets.

Overall, the loop-source transient electromagnetic method demonstrates strong applicability for detecting subglacial hydrological systems in polar regions. It exhibits significant detection potential for identifying low-resistivity anomalies associated with fluid activity and potential mineralization within thickly covered environments.These findings provide valuable technical references for subglacial hydrological investigations, deep geological structure studies, and deep mineral exploration in polar regions and other areas characterized by thick resistive cover.

How to cite: Zhang, Y., Zou, C., Boaga, J., and Peng, C.: Transient electromagnetic responses to deep low resistivity targets beneath thick resistive ice sheet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17065, https://doi.org/10.5194/egusphere-egu26-17065, 2026.

EGU26-17188 | ECS | PICO | CR6.2

Passive Radar Sounding of Firn Aquifers: Geophysical Constraints and Sensitivity 

Sean Peters, Angela Wang, Nainika Gupta, and Riley Culberg

Firn aquifers retain liquid meltwater within the near-surface layers of ice sheets and ice shelves, which may influence mass balance and subglacial hydrology. Despite their importance, measuring changes in firn aquifer water storage remains a challenge using existing satellite, airborne, and ground-based active radar methods, largely due to the significant spatial and temporal variability of firn aquifers. Complementary to active radar techniques, passive radar sounding is an advancing radioglaciological method that does not transmit its own signal for echo detection, but instead receives and correlates ambient radio emissions from the Sun to detect subsurface reflections, including those from firn aquifers.

In this presentation, we investigate the geophysical constraints (e.g., firn temperature, saturation, density, and depth) that govern the sensitivity of passive radar sounding to detect firn aquifer water table fluctuations. Our analysis highlights simulation-based, site-specific case studies representative of firn aquifer environments in Greenland, Svalbard, and Antarctica. Using realistic firn properties and expected solar geometry throughout the year, we evaluate signal attenuation, depth sensitivity, and expected echo time delays to identify seasonal observation windows for passive sounding.

Our results show that passive radar sounding can achieve sufficient signal-to-noise ratio and depth sensitivity to support monitoring on daily to seasonal timescales, particularly during and after the summer melt season when the most rapid changes in firn aquifers are likely to occur. These results further highlight the conditions under which passive sounding could enable quasi-continuous monitoring of firn aquifer dynamics and address a key gap in current cryospheric observational strategies.

How to cite: Peters, S., Wang, A., Gupta, N., and Culberg, R.: Passive Radar Sounding of Firn Aquifers: Geophysical Constraints and Sensitivity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17188, https://doi.org/10.5194/egusphere-egu26-17188, 2026.

EGU26-17761 | PICO | CR6.2

Resistivity vs Temperature Laboratory Experiments on Arctic Sediments: Quantifying the Effects of Texture, Salt, and Cryostructure  

Saskia Eppinger, Julius Kunz, Maike Offer, Michael Angelopoulos, Michael Fritz, Pier Paul Overduin, and Michael Krautblatter

When investigating Arctic permafrost sediments, Electrical Resistivity Tomography (ERT) is becoming increasingly popular due to its robust, relatively quick and non-invasive application. The interpretation of ERT data is often constrained by the knowledge of the geophysical properties of the encountered frozen materials, thereby highlighting the need for ERT calibration experiments. Lab experiments on samples can quantify the dependency of electrical resistivity on sediment temperatures. Variation in electrical resistivity also depends on sediment composition, ground ice structures and their orientation with respect to the array, and porewater chemistry, all of which need to be considered in interpreting field measurements.

This study aims to improve our interpretation of ERT field measurements by investigating controlling and limiting factors of validating measurements by laboratory tests. We performed these laboratory tests on synthetic mixtures and field samples, varying sample size, electrode array orientation, electrode spacing, electrode type and anisotropy. Samples were thawed and then refrozen during the tests to include hysteresis effects. Synthetic samples were built to provide known anisotropies. Field samples were used from sites in Canada, and on Greenland and Svalbard. Relationships between apparent electrical resistivity and temperature were compared with hydro-chemical analyses of sediment porewater, grain size and ice content.

The tests on artificial samples helped improving our experiment design and highlighted the importance of anisotropy in comparison with the effects spacing or sample sizes. The field samples showed the importance of ice content and cryostructures as well as high salt content on the temperature-resistivity curves. Our research enables a better understanding of the temperature-resistivity dependency, provides information on sample sizes and anisotropy limitations necessary for fieldwork sampling, and overall allows for a better understanding and therefore interpretation of temperature dependent ERT datasets.

How to cite: Eppinger, S., Kunz, J., Offer, M., Angelopoulos, M., Fritz, M., Overduin, P. P., and Krautblatter, M.: Resistivity vs Temperature Laboratory Experiments on Arctic Sediments: Quantifying the Effects of Texture, Salt, and Cryostructure , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17761, https://doi.org/10.5194/egusphere-egu26-17761, 2026.

EGU26-17913 | ECS | PICO | CR6.2

Using UAV-based 4D GPR to investigate the seasonal and interannual evolution of englacial and subglacial drainage 

Johanna Klahold, Gabriela Clara Racz, Bastien Ruols, and James Irving

Meltwater routing through englacial and subglacial drainage systems exerts a fundamental control on glacier dynamics, water resources, and related hazards, yet detailed observations of these systems and their temporal evolution remain scarce. In this study, we present uncrewed aerial vehicle (UAV)-based four-dimensional (4D) ground-penetrating radar (GPR) measurements that resolve seasonal and interannual changes in near-terminus glacier hydrology at unprecedented spatial resolution.

We conducted repeated high-density 3D GPR surveys at the Otemma Glacier (Swiss Alps) during four field campaigns (August 2022; June, August, and October 2023). A dedicated 3D processing workflow combining reflection-based imaging of the glacier bed with coherence-based diffraction imaging of englacial scatterers enables comparison of drainage structures across surveys. The GPR results are interpreted alongside complementary observations, including dye tracing experiments, UAV photogrammetry, time-lapse imagery, and a targeted steam drill validation.

Our results reveal a drainage system composed of both persistent and dynamically reorganizing components. Subglacially, one major conduit remains stable across years and shows signs of increasing hydraulic efficiency, while a second conduit is partly rerouted. Englacially, several channels are observed in similar locations across years, indicating structural persistence, whereas other features appear transient. Seasonal drainage evolution is evident, and we observe direct coupling between englacial and subglacial drainage systems manifested by co-evolving structural changes.

These observations demonstrate the potential of UAV-based 4D GPR to capture glacier hydrological dynamics and provide critical constraints for models of meltwater routing and ice dynamics under a changing climate.

How to cite: Klahold, J., Racz, G. C., Ruols, B., and Irving, J.: Using UAV-based 4D GPR to investigate the seasonal and interannual evolution of englacial and subglacial drainage, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17913, https://doi.org/10.5194/egusphere-egu26-17913, 2026.

EGU26-18959 | ECS | PICO | CR6.2

Seismic evidence for frictional heterogeneity and transient basal slip beneath a fast Greenland outlet glacier 

Ana Nap, Thomas S. Hudson, Fabian Walter, Adrien Wehrlé, Andrea Kneib-Walter, Hugo Rousseau, and Martin P. Lüthi

Basal friction and stick–slip processes beneath fast-flowing glaciers play a key role in modulating ice dynamics, yet the physical conditions at the ice–bed interface remain poorly constrained. Here, we use seismic observations of basal icequakes recorded within the ice stream of a fast-flowing Greenland outlet glacier to investigate frictional heterogeneity and transient slip behavior at the glacier bed. Using a three-sensor seismic array, we detect nearly 25,000 short-duration seismic events over 5-week period that occur in spatially coherent clusters, indicating repeated failure on localized basal asperities.

We analyze S-wave spectra within these clusters using the Brune source model and interpret the results within a rate-and-state friction framework to estimate relative variations in basal frictional stress through space and time. Our analysis reveals pronounced heterogeneity in basal seismic slip and stress behavior, with one persistent, spatially extensive region exhibiting systematically higher inferred frictional stresses throughout the observation period. This suggests that basal friction is not spatially uniform but instead governed by a patchwork of asperities that repeatedly load and fail, including at least one long-lived, dominant “sticky-spot”.
In addition to this localized behavior, we observe kilometre-scale downstream and upstream migration of icequake activity. These migration patterns suggest the presence of transient, propagating slip fronts, analogous to faster slip behavior previously observed beneath the Whillans Ice Stream, Antarctica, as well as in some tectonic fault systems. The inferred slip fronts propagate faster than glacier flow speeds and show a weak correlation with the tidal signal at the glacier terminus, indicating that their evolution might be controlled by small external stress changes.

Together, these observations support a view of glacier basal motion as a highly dynamic and locally controlled process rather than a spatially averaged frictional regime. The additional evidence for seismic migration highlights an interplay between localized stress accumulation at persistent asperities and more distributed, evolving slip processes, both of which may influence the dynamics and stability of fast glacier flow.

How to cite: Nap, A., Hudson, T. S., Walter, F., Wehrlé, A., Kneib-Walter, A., Rousseau, H., and Lüthi, M. P.: Seismic evidence for frictional heterogeneity and transient basal slip beneath a fast Greenland outlet glacier, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18959, https://doi.org/10.5194/egusphere-egu26-18959, 2026.

EGU26-19320 | PICO | CR6.2

Mass Change of the North West Sector of the Greenland Ice Sheet during 1900-2025 

Tobias Socher, Shfaqat Abbas Khan, and Anders Anker Bjørk

The Greenland Ice Sheet is currently the largest single land-ice contributor to global sea level rise, and this contribution is expected to continue throughout the twenty-first century and beyond, although the magnitude and rate of future mass loss remain highly uncertain. A key limitation in current estimates is that most observational records span only the last few decades, providing an incomplete view of long-term glacier behavior. Improving future projections therefore requires a better understanding of how Greenland's outlet glaciers have responded to external climate forcing over centennial timescales. In this study, we combine historical aerial and ground-based photographs with modern satellite observations to reconstruct ice-sheet change from approximately 1900 to 2025 in the northwest sector of the Greenland Ice Sheet, spanning from Jakobshavn Isbræ in the south to the outlet glaciers of Melville Bugt in the north. Using these complementary datasets, including satellite altimetry, ice-flow maps, and terminus positions, we quantify ice loss, surface elevation change, frontal retreat, and ice dynamics for three major outlet glaciers. The observations provide new insight into the processes driving glacier evolution and their contribution to future sea level rise.

How to cite: Socher, T., Khan, S. A., and Bjørk, A. A.: Mass Change of the North West Sector of the Greenland Ice Sheet during 1900-2025, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19320, https://doi.org/10.5194/egusphere-egu26-19320, 2026.

EGU26-19533 | PICO | CR6.2

Shifting the Metric from Overlap to Information Density – Improved UAV Photogrammetry Strategies for High-Alpine Snow Depth Mapping 

Jakob Knieß, Paul Schattan, Franziska Koch, and Karl-Friedrich Wetzel

Abstract:
Knowledge of spatio-temporal snow storage is crucial to understand snow-hydrological dynamics in complex, high alpine environments. Due to the low cost and fast deployability, photogrammetry in combination with commercial aerial photography UAVs has become a viable method for capturing high-resolution snowpack information. We utilize this technique in a high alpine catchment at Mt. Zugspitze in Germany to capture digital snow surface models and consequently snow depth information in heterogeneous environments. The fundamental step is the acquisition of overlapping aerial images, which are used for the reconstruction of the surface in the photogrammetric processing. It is well known that the properties of the image dataset determine the quality of the resulting reconstruction. Therefore, a number of studies from different areas of research focus on this topic. For snow depth mapping, Bühler et al. 2016 recommend, for instance a single overlap value, while Lee et al. 2021 collected different overlap values. Wu et al. 2025 found that the 3D model quality in an urban environment is linked to the overlap of an oblique image dataset in a nonlinear way. Depending on the studied terrain and structures, Maes 2025 summarizes various recommendations for appropriate overlap settings. To provide an insight into how often, in what resolution, and from which angle an area is captured, the current concept of overlap is unsuited. We suggest a paradigm change towards metrics representing the image information of a surface. Our approach is to increase the image capture frequency while angling the camera in a forward direction, wherefore a high image capture frequency of current digital camera systems is fundamental. Through this combination, the near-nadir information is retained, and the changed viewing geometry provides additional information in the along path and side view directions. The potential can be used for an increase in the dataset quality or a decrease in capture time. Both are highly relevant when working in the structurally complex and remote regions of high mountain areas. Battery capacity and regulations for flight speed and height do limit other options for an increase in data capture. Our goal is to share preliminary results for increasing the information in the image dataset while staying within the capability of current hardware.

Literature:

Bühler, Y., Adams, M.S., Bösch, R., Stoffel, A., 2016. Mapping snow depth in alpine terrain with unmanned aerial systems (UASs): potential and limitations. The Cryosphere 10, 1075–1088. https://doi.org/10.5194/tc-10-1075-2016

Lee, S., Park, J., Choi, E., Kim, D., 2021. Factors Influencing the Accuracy of Shallow Snow Depth Measured Using UAV-Based Photogrammetry. Remote Sensing 13, 828. https://doi.org/10.3390/rs13040828

Maes, W.H., 2025. Practical Guidelines for Performing UAV Mapping Flights with Snapshot Sensors. Remote Sensing 17, 606. https://doi.org/10.3390/rs17040606

Wu, S., Feng, L., Zhang, X., Yin, C., Quan, L., Tian, B., 2025. Optimizing overlap percentage for enhanced accuracy and efficiency in oblique photogrammetry building 3D modeling. Construction and Building Materials 489, 142382. https://doi.org/10.1016/j.conbuildmat.2025.142382

How to cite: Knieß, J., Schattan, P., Koch, F., and Wetzel, K.-F.: Shifting the Metric from Overlap to Information Density – Improved UAV Photogrammetry Strategies for High-Alpine Snow Depth Mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19533, https://doi.org/10.5194/egusphere-egu26-19533, 2026.

EGU26-19928 | PICO | CR6.2

Measurements of shear and stress at Bowdoin Glacier, Northwest Greenland 

Julien Seguinot, Evgeny A. Podolskiy, Katarina Henning, Shin Sugiyama, Ralf Greve, and Harry Zekollari

Englacial stress, the elusive variable governing glacier motion, has rarely been measured in situ. Instead, our empirical understanding of ice dynamics largely relies on laboratory flow-law experiments, but field measurements of stress-induced glacier surface velocity and englacial tilt indicate that crystal orientation, molten ice fraction and impurities may complicate the application of laboratory-derived laws in nature. Here, we present a three-year record of englacial deformation and near-vertical stress from sensors frozen 123 to 265 metres deep into the Bowdoin tidewater glacier in Northwest Greenland.

Inclinometers show that the glacier movement is largely dominated by sliding, as horizontal shear deformation of 16 to 19 metres accounts for 4 to 5 percent of independently observed surface displacement. During seasonal speed-up events, englacial tilt rates increase proportionally to surface velocities derived from geopositioning, automated cameras and satellite remote sensing. Daily and tidal components are also present in the tilt rates record but are yet to be isolated from the sampling noise before phase correlation with other signals.

Piezometers were initially intended to locate instruments in hotwater-drilled boreholes, but they continued to record pressure changes after the complete refreezing of the boreholes and the stabilisation of ice temperatures well below the melting point. All sensors recorded in-phase stress variations with 12-hour, 24-hour and 14-day periodicities, revealing a tidal signal in winter, disturbed during independently documented speed-up events in summer. The signal shows amplitudes of one to four kilopascals, only an order of magnitude weaker than the two metres tidal amplitude measured at sea. However, stress measurements are anticorrelated with the tide, and show a delay of one to two hours, so that maximum stresses occur a little after low tide. While detailed interpretations are hampered by the lack of calibration, our data indicate that direct stress measurements in glaciers are feasible.

How to cite: Seguinot, J., Podolskiy, E. A., Henning, K., Sugiyama, S., Greve, R., and Zekollari, H.: Measurements of shear and stress at Bowdoin Glacier, Northwest Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19928, https://doi.org/10.5194/egusphere-egu26-19928, 2026.

EGU26-20650 | PICO | CR6.2

Distinct Groundwater Regimes in West Antarctic Sedimentary Basins Inferred from Magnetotelluric Imaging. 

Siobhan Killingbeck, Bernd Kulessa, Rebecca Pearce, Alex Brisbourne, Louise Borthwick, Felipe Napoleoni, Sridhar Anandakrishnan, Martyn Unsworth, and Atsuhiro Muto

Subglacial sedimentary basins in Antarctica are hypothesized to modulate ice flow and biogeochemical cycles via groundwater and geothermal feedbacks, yet their properties remain poorly constrained. As part of the International Thwaites Glacier Collaboration’s (ITGC) GHOST project, we acquired new magnetotelluric (MT) geophysical data on Thwaites Glacier (TG) and at the West Antarctic Ice Sheet (WAIS) Divide during the 2022/23 and 2023/24 austral summers.

These new data are integrated with an archive of existing MT profiles from the Whillans Ice Stream, Central West Antarctica, the South Pole, and the Ross Ice Shelf to provide a continent-scale perspective. Using a constrained 1-D transdimensional Bayesian inversion, we produce new depth-resistivity models for the uppermost crust beneath the ice at each location, and interpret these models in terms of geological, geothermal and hydrogeological conditions beneath each profile.

The new MT data reveal a shallow (< 5 km) 2-D crustal structure at TG aligned with the West Antarctic Rift System, overlying deeper 3-D architectures potentially linked to older tectonic frameworks, e.g., the Weddell Sea Rift System. Our inversion highlights that the sedimentary basin beneath TG exhibits relatively high resistivity (>10 Ωm), distinct from the low-resistivity (<10 Ωm) basins observed beneath the Whillans Ice Stream, South Pole and Ross Ice Shelf. Sensitivity analysis reveals that the TG basin is horizontally heterogeneous, with conductive signatures in thicker sections and resistive, potentially low porosity, fresh conditions at GHOST Ridge, a subglacial topographic high which has been identified as a potential future stabilizing point. Conversely, basins beneath Subglacial Lake Whillans and the South Pole exhibit vertical stratification, likely hosting fresh, cold upper layers above deep, saline, and potentially warm reservoirs.

We conclude that complex, spatially variable groundwater regimes are widespread in Antarctica. These contrasting hydrological environments imply continent-scale variability in subglacial thermodynamics and ice dynamics. Furthermore, they suggest spatially distinct biogeochemical potentials, influencing subglacial carbon sequestration and the rates of dissolved carbon discharge into the Southern Ocean.

How to cite: Killingbeck, S., Kulessa, B., Pearce, R., Brisbourne, A., Borthwick, L., Napoleoni, F., Anandakrishnan, S., Unsworth, M., and Muto, A.: Distinct Groundwater Regimes in West Antarctic Sedimentary Basins Inferred from Magnetotelluric Imaging., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20650, https://doi.org/10.5194/egusphere-egu26-20650, 2026.

EGU26-21527 | ECS | PICO | CR6.2

Direct Ice Density Constraints from Multimode Surface Waves Using DAS 

Ariane Lanteri, Scott Keating, Lars Gebraad, Sara Klaasen, Marta Pienkowska-Cote, Olaf Eisen, Andrea Zunino, Kristin Jonsdottir, Coen Hofstede, Dimitri Zigone, and Andreas Fichtner

Constraining subsurface density from seismic data is challenging, although density is fundamental to quantifying mass and structure in both the solid Earth and glaciers. Empirical scaling relationships between seismic wave speeds and density are therefore widely used. In this contribution, we show that density can instead be constrained directly from surface-wave observations when multimode dispersion and fully nonlinear inversion are combined.

We analyze distributed acoustic sensing (DAS) recordings acquired in glaciated environments, where strong serendipitous anthropogenic sources generate coherent Rayleigh-wave overtones with high signal-to-noise ratio. These dense DAS measurements allow robust extraction of surface-wave multimode dispersion. We invert the data using a probabilistic Hamiltonian Monte Carlo (HMC) framework that accounts for nonlinearity, parameter trade-offs, and uncertainty, while avoiding biases introduced by subjective regularization choices.

Our results show that Rayleigh-wave overtones carry resolvable sensitivity to density structure down to depths of order 100 m, enabling direct density estimation from seismic data with quantified uncertainties. We further evaluate commonly used velocity–density scaling relationships for firn (the transitional layer between fresh snow and glacial ice) and find that their application can lead to density errors on the order of 10%, with direct implications for inferred mass estimates.

Overall, these findings demonstrate that overtone-based probabilistic inversion enables constraints on weakly sensitive parameters and highlight the potential of DAS for quantitative near-surface parameter estimation.

How to cite: Lanteri, A., Keating, S., Gebraad, L., Klaasen, S., Pienkowska-Cote, M., Eisen, O., Zunino, A., Jonsdottir, K., Hofstede, C., Zigone, D., and Fichtner, A.: Direct Ice Density Constraints from Multimode Surface Waves Using DAS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21527, https://doi.org/10.5194/egusphere-egu26-21527, 2026.

EGU26-879 | ECS | Posters on site | CR6.3

 PANTHER – First experimental demonstration of using Jovian radio bursts as an illuminator of opportunity for passive radar echo detection 

Thorsteinn Kristinsson, Sean Peters, Joana Voigt, Gregor Steinbrugge, Christopher Hamilton, Serina Diniega, Jonathan Williams, Gustavo Alfonso, and Andrew Romero-Wolf

The use of astronomical radio sources has been demonstrated for sounding and echo detection using quiescent solar emissions in VHF (300 MHz). Here, we present the first demonstration of using Jovian HF radio bursts (25 MHz) to detect a reflection off the hills of Dante’s View in Death Valley, California.

Solar emissions are governed by blackbody radiation, which at HF is not resolvable from the galactic background noise. In contrast, Jovian bursts are governed by the interaction of Jupiter’s magnetosphere and Io’s magnetic field, which produces a significantly stronger and detectable HF emission on Earth, Mars, and Europa. While this mechanism is not continuous, it is highly predictable, as the orbital parameters of Jupiter System III central meridian longitude and Io’s orbital phase dictate the probability of a burst occurring.

As part of the Passive Autonomy, Navigation, Topography, and Habitability Exploration Radar (PANTHER), our system setup uses an HF dipole antenna and software-defined radio (Ettus X310 TwinRX) to receive radio signals at a 25 MHz center frequency with a 20 MHz bandwidth. The expectation of the experiment was to observe the reflection of a Jovian burst from Badwater Basin, which behaves like a flat specular reflector. However, during the field demonstration, the timing of the bursts—combined with Jupiter’s elevation angle and viewing geometry from Dante’s View—did not produce a basin reflection. Instead, this experiment required a more complex geometric analysis and signal processing to determine a reflection point on the hillside of Dante’s View. We emphasize that demonstrations using Jovian bursts thus require additional geometric and timing constraints that were not required for prior passive sounding experiments using continuous quiescent solar emissions. In addition to predicting the burst windows, this technique requires selecting an antenna location that provides favorable reflection geometry.

Our results provide the first demonstration of a Jovian radio burst as an HF source for passive radar echo detection, which is the first step towards a low-resource passive HF system that uses Jovian bursts for future planetary sounding missions. Building on this first demonstration, PANTHER aims to utilize the benefits of the HF signal and its lower attenuation coefficient to sound geologic targets in Iceland including glaciers, lava flow fields, and subsurface ice deposits.

How to cite: Kristinsson, T., Peters, S., Voigt, J., Steinbrugge, G., Hamilton, C., Diniega, S., Williams, J., Alfonso, G., and Romero-Wolf, A.:  PANTHER – First experimental demonstration of using Jovian radio bursts as an illuminator of opportunity for passive radar echo detection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-879, https://doi.org/10.5194/egusphere-egu26-879, 2026.

EGU26-1380 | ECS | Orals | CR6.3

A radar equation for snow-covered targets in radar altimetry 

Hoyeon Shi and Rasmus Tonboe

Waveform simulators are commonly used to retrack ice surface elevations from radar altimeter observations. Most simulators apply the radar equation to estimate backscattered power, but this formulation often overlooks refraction at the snow surface. Because snow alters the propagation direction of the radar pulse, refraction modifies both the incidence angle and the geometry of the propagating wavefront.

In this study, we derived a modified radar equation for snow-covered ice surfaces that explicitly accounts for refraction. Implementing this formulation within a waveform simulator produces waveforms that are systematically dampened and broadened relative to those generated using the conventional radar equation. Two main mechanisms account for these differences: (1) changes in wavefront geometry that reduce the returned power by a factor proportional to the square of the snow's refractive index, and (2) decreased incidence angles that increase the returned power at increasing off-nadir distances.

Our results suggest that neglecting refraction in waveform-simulator-based retracking can introduce biases in track points, as the retracker may compensate for unmodeled refraction by overestimating surface roughness. These findings underscore the importance of incorporating refraction into radar altimetry forward models to achieve accurate measurements over snow-covered ice.

How to cite: Shi, H. and Tonboe, R.: A radar equation for snow-covered targets in radar altimetry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1380, https://doi.org/10.5194/egusphere-egu26-1380, 2026.

In the western Greenland ablation zone, most meltwater is thought to drain to the bed of the ice sheet through moulins or hydrofractures, leading to surface mass loss and seasonal ice velocity variations. However, there is a growing body of work on slow and partial depth hydrofracture, which could store meltwater englacially for longer periods of time. If widespread, this process would reduce total surface mass loss from the ablation zone, delay or reduce meltwater delivery to the subglacial system, and warm the ice through latent heat release, thus modulating all aspects of glacier mass balance.

Here, we investigate a spatially extensive, non-conformal englacial volume scattering horizon observed in Operation IceBridge ice-penetrating radar data collected in the springs of 2011-2019 in the western Greenland ablation zone. The depth of this horizon coincides with thermal anomalies in borehole temperature profiles, suggesting that it may be evidence of englacial liquid water pockets. We test this hypothesis in the Sermeq Avannarleq catchment using a Mie scattering model and show that the radar reflectivity and attenuation of this horizon are most consistent with scattering from sparse, meter-scale water inclusions in a layer of macro-porous ice ~60-80 m thick. These inversion results suggest that around 0.8 m/m2 of liquid water are stored over winter in the bottoms of surface crevasses at this site. At this same site, we also show that interannual variability in the attenuation anomaly from the scattering horizon is highly correlated with the preceding summer’s melt volume, providing further evidence linking this structure to water storage. Finally, we map the extent of this scattering horizon across the western Greenland ablation zone and find extensive spatial coverage in almost every glacier catchment from 60°-77° N. Our results show that englacial water storage is likely ubiquitous in the western Greenland ablation zone and therefore may play a more important role in modulating englacial temperature, surface mass balance, and subglacial drainage than previously assumed.

How to cite: Culberg, R. and Seleen, C.: Radar Evidence for Widespread Englacial Over-Winter Water Storage in Greenland’s Ablation Zone, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2010, https://doi.org/10.5194/egusphere-egu26-2010, 2026.

EGU26-8480 | ECS | Posters on site | CR6.3

3D full-waveform inversion of asteroid interior from monostatic radar data and its implications for acquisition geometry optimization 

Zhiwei Xu, Yuefeng Yuan, Peimin Zhu, Fenghzu Zhang, Shi Zheng, Ruidong Liu, and Shuanlao Li

Understanding the interior structure and lithology of asteroids is crucial for gaining insights into their origin and evolution. The European Space Agency’s (ESA) Hera and China’s Tianwen-2 asteroid missions will employ monostatic orbital radar to investigate the interiors of the target asteroids Dimorphos and 2016 HO3, respectively. While most previous studies have focused on imaging asteroid interiors using bistatic radar data, relatively few have explored the same task using monostatic radar data (MRD). To support the measurement strategy and upcoming data processing for the two missions, it is essential to investigate potential imaging methods for reconstructing asteroid interiors from MRD. In this study, we propose a three-dimensional (3D) full-waveform inversion (FWI) approach to obtain the internal structure and permittivity distribution from MRD. Numerical experiments on 3D rubble pile and onion shell asteroid models validate the feasibility and accuracy of the proposed method. Additionally, a sensitivity analysis is performed using the 3D onion shell model to assess the influence of three factors—radar measurement points, number of orbits, and distance between adjacent orbits—on the FWI results. This study offers an effective approach for imaging asteroid interiors using MRD and provides valuable insights for optimizing acquisition geometries in future asteroid missions.

How to cite: Xu, Z., Yuan, Y., Zhu, P., Zhang, F., Zheng, S., Liu, R., and Li, S.: 3D full-waveform inversion of asteroid interior from monostatic radar data and its implications for acquisition geometry optimization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8480, https://doi.org/10.5194/egusphere-egu26-8480, 2026.

EGU26-9941 | ECS | Orals | CR6.3

 Simulation-based inference of depth-resolved radar attenuation rates  

Leah Sophie Muhle, Guy Moss, Rebecca Schlegel, and Reinhard Drews

Radar attenuation rates are required to infer basal properties, to identify subglacial water and to characterise the thermal state of ice sheets. However, existing methods of estimating attenuation rates from radar measurements only provide depth-averaged values and rely on simplifying assumptions such as spatially constant reflectivity along the bed reflector or near-constant reflectivity of internal reflection horizons (IRHs) within the ice column. Comparisons of these methods on the same radar data set clearly show that depth-averaged attenuation rate estimates are strongly method-dependent and exhibit significant biases, which hinder the full interpretation of radar data.

Here, we present a novel approach that provides improved depth-averaged attenuation rate estimates and, unlike previous works, can estimate depth-resolved attenuation rate profiles. We cast the problem of estimating attenuation rates as a Bayesian inference problem. To solve for the posterior distribution of attenuation rates underlying radar data, we first design a radar forward model that can generate realistic radar traces given depth profiles of attenuation rates. Subsequently, we apply Neural Posterior Estimation, a machine learning technique for estimating Bayesian posterior distributions, and train it on pairs of simulated radar traces and attenuation rate profiles. For synthetic radar data, our approach robustly infers both depth-averaged and depth-resolved attenuation rates and outperforms existing methods. We further demonstrate its transferability to ground-penetrating radar data collected at two distinct ice-dynamic settings in Antarctica: South Pole Lake and Rutford Ice Stream. In both cases, the temperature profiles derived from the inferred depth-resolved attenuation rates match in-situ borehole temperature measurements. This is a significant step forward in recovering englacial temperatures from ground-penetrating radar data, as well as in achieving an uncertainty-constrained interpretation of the basal reflection power. 

How to cite: Muhle, L. S., Moss, G., Schlegel, R., and Drews, R.:  Simulation-based inference of depth-resolved radar attenuation rates , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9941, https://doi.org/10.5194/egusphere-egu26-9941, 2026.

Satellite remote sensing is the primary way to monitor seasonal as well as long-term changes across broad portions of the Arctic. Subject to certain conditions (e.g., illumination), these data are collected continuously with known spatiotemporal coverage and resolution. And when supplemented with ground-based in situ calibration/validation measurements, satellite measurements can be used to infer some of the critical geophysical properties (e.g., surface elevation change, surface melting, etc.) that underpin our ability to project long-term ice sheet and ice cap evolution to in the future.

 This workflow however relies on the assumption that how the actual in situ conditions affect and manifest within the satellite measurements is constant or predictable through time and space. Put another way, that the in situ measurements used in calibration and validation are 1) representative of all transient (e.g., seasonal and/or multi-annual) conditions, or 2) that we can reliably modify/correct our satellite data interpretations to account for these changes. Recent work on the Greenland Ice Sheet has started to show that this assumption may be violated during periods of extreme warming; where warming may impact the satellite measurements in one way in one region (e.g., as an increase in radar altimetry echo strength), but in a different way in another (e.g., a fall in radar altimetry echo strength). Without a fuller understanding of how melting is affecting the ice sheet near-surface, these differences directly complicate the recovery of temporally comparable long-term satellite records.

 As an alternative to costly in situ calibration/validation campaigns, in this study we investigate the transient changes in the surface conditions of Arctic ice caps (i.e., Flade Isblink in Greenland, Austfonna in Svalbard and Vatnajökull in Iceland) via their impact on multiple satellite datasets. Small Arctic ice caps are useful in this regard as they often experience more variable climate forcings than remote interior portions of the Greenland Ice Sheet and therefore stronger seasonal patterns. Specifically, we are interested in developing a consistent model for how seasonal melt alters the near-surface of these ice caps by integrating Copernicus Sentinel-2 (optical), ESA CryoSat-2 (Ku-band radar altimetry), ISRO/CNES SARAL/AltiKa (Ka-band radar altimetry), Copernicus Sentinel-1 (C-band SAR), ESA SMOS (L-band passive microwave), and JAXA AMSR-2/E (multi-frequency passive microwave) satellite datasets. Our interpretation of these satellite datasets are supplemented with in situ measurements where available.

How to cite: Scanlan, K. M.: Unravelling Seasonal Changes in Arctic Ice Cap Surface Conditions through Multi-Satellite Synthesis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10425, https://doi.org/10.5194/egusphere-egu26-10425, 2026.

EGU26-12953 | Posters on site | CR6.3

Anomalous Shallow Subsurface Radar Reflections Detected by MARSIS in the South Polar Layered Deposits 

Andrea Cicchetti, Roberto Orosei, Elena Pettinelli, Sebastian Lauro, Raffaella Noschese, and Marco Cartacci

Analysis of Flash Memory [1] data acquired by the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) instrument aboard ESA’s Mars Express spacecraft, confirms the presence of additional strong subsurface reflections within the South Polar Layered Deposits, located near the northernmost extent of the previously identified subglacial water bodies [2,3].
Figure 1 shows the ground track of orbit 10786 over the topography of the Martian South Pole, where anomalous subsurface reflections have been recorded, highlighted by the blue dots.

 

Fig. 1. Topography Maps of the investigated area.

The ground track of orbit 10786 (Figure 2, panel a) crosses the Martian south polar region where these anomalous reflections are detected at shallow depths, occurring approximately 5μs after the surface echoes. A comparison between the observed radar signals and electromagnetic simulations of surface returns (Figure 2, panels b and d) demonstrates that these features are authentic subsurface reflections rather than lateral clutter. The analysis of surface and subsurface echo power (Figure 2, panel e) reveals that, in several signals, the subsurface echoes are significantly stronger than the corresponding surface echoes, indicating a pronounced dielectric contrast variation, between the overlying medium and the subsurface target. Constraining the dielectric properties and the nature of the subsurface material, requires further investigation. This effort will be supported by future MARSIS observations planned for August 2027 and, in particular, April 2029, when the instrument will observe the region during the deep Martian night, thus minimizing ionospheric attenuation and distortion effects.

Fig. 2. Science Investigation. a) Zoom of the topography map. b) Comparison between real and simulated data at echo level. c) Simulated Radargram. d) Real data. e) Trends of surface and subsurface echo power.

References:
[1] A. Cicchetti, et al., Observations of Phobos by the Mars Express radar MARSIS: Description of the detection techniques and preliminary results. Adv. Space Res. 60, 2289-2302 (2017).
[2] Orosei R. et al., “Radar evidence of subglacial liquid water on Mars”, 2018, Science, 361
[3] Lauro S.E. et al., “Multiple subglacial water bodies below the south pole of Mars unveiled by new MARSIS data”, 2022, Nature Astronomy


This work was supported by the Italian Space Agency (ASI) through contract 2024-40-HH.0

How to cite: Cicchetti, A., Orosei, R., Pettinelli, E., Lauro, S., Noschese, R., and Cartacci, M.: Anomalous Shallow Subsurface Radar Reflections Detected by MARSIS in the South Polar Layered Deposits, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12953, https://doi.org/10.5194/egusphere-egu26-12953, 2026.

EGU26-14142 | Posters on site | CR6.3

A compact FMCW Radar as a Proximity Sensor and Subsurface Analyzer for Landers or CubeSats in Planetary or Small Body Missions 

Dirk Plettemeier, Martin Laabs, and Fabian Geißler

Planetary and small-body lander missions, as well as CubeSat-based exploration platforms, require robust proximity sensing capabilities to support descent, landing, and surface operations. This contribution presents a compact, coherent dual-channel FMCW radar designed as a proximity sensor for planetary and small-body missions. The radar features a volume of less than half a CubeSat unit and operates over a wide, mission-configurable frequency range from 10 MHz to 6 GHz, allowing adaptation to antenna accommodation, platform constraints, and planetary protection or regulatory requirements. The integrated power amplifier provides a transmit power of up to 2 W, while the minimum detectable signal reaches −125 dBm. Output power and sensitivity can be further extended using external amplification stages if required.

The radar is fully software-configurable, offering flexible control over RF bandwidth, sweep duration, intermediate-frequency sampling rate, and output power. It supports up to two transmit and two fully independent, phase-coherent receive channels. Depending on the operational duty cycle, average power consumption can be as low as 2.5 W, making the system suitable for resource-constrained CubeSat and lander platforms.

Designed for autonomous operation, the system performs real-time, on-board signal processing to provide deterministic, terrain-relative proximity measurements independent of external navigation or communication infrastructure. In its primary mode, the radar functions as a radar altimeter and descent monitor, delivering continuous estimates of range to the surface and relative vertical velocity. These measurements are well suited for guidance, navigation, and control during terminal descent, landing detection, and post-landing assessment.

In secondary mode, the radar can be used as a surface analyzer and subsurface sounder. Due to its enormous bandwidth and high dynamic range, the radar can be operated as a surface analyzer to map surface permittivity and roughness and, in GPR mode, to characterize the shallow subsurface with high spatial resolution. In the low-frequency range, the instrument is capable of performing deep sounding measurements with high penetration depth to analyze the deep interior of small bodies or planetary subsurface structures.

In addition, a cooperative transponder mode enables two-way FMCW ranging between multiple mission elements, such as a lander and an accompanying CubeSat or orbiter, supporting relative navigation and formation tracking. Operating at low frequencies with link budgets of up to approximately 155 dB, this mode allows the use of simple, non-directional antennas. A low-data-rate communication mode can also be implemented on the same hardware to support beaconing and basic command and housekeeping functions during descent and surface operations.

The presented radar system is intended as mission-agnostic proximity-sensing infrastructure for planetary exploration. Owing to its coherent architecture, it is inherently compatible with advanced processing techniques, including synthetic aperture processing for surface characterization and subsurface sounding, which are identified as promising directions for future work.

How to cite: Plettemeier, D., Laabs, M., and Geißler, F.: A compact FMCW Radar as a Proximity Sensor and Subsurface Analyzer for Landers or CubeSats in Planetary or Small Body Missions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14142, https://doi.org/10.5194/egusphere-egu26-14142, 2026.

EGU26-14385 | ECS | Orals | CR6.3

Preliminary tests to combine X-ray microtomography and dielectric measurements to assess the radar properties of pure water ice 

Flavia Cimbolli Spagnesi, Barbara Cosciotti, Sebastian Emanuel Lauro, Elisabetta Mattei, and Elena Pettinelli

Two large space missions, JUICE and EUROPA Clipper are on their way to reach the icy satellites of Jupiter in the early 2030s. One of the main scope of these missions is to find liquid water below/inside the icy crusts and to assess the habitability conditions of such ocean worlds. Radar sounders, on board these missions, will play a fundamental role in detecting position, depth and composition of the water. However, presently our understanding of the composition and thermal state of such icy crusts is poorly constrained, which makes the detection of liquid water using radio waves very difficult. Therefore, it is of paramount importance to perform systematic measurements of the dielectric properties of a large set of icy materials having different salt composition and temperature, to define the range of penetration of the radar signals in different scenarios and to assess the detectability limit of the water.

To reach this goal, as a first step, it is important to determine the dielectric properties of pure water ice in the frequency range typical of planetary radar sounders (1-100 MHz). The aim of this work was to optimize the laboratory procedure to assess such properties, combining X-ray micro-computed tomography images with low/high frequency dielectric measurements. The experimental activity was first focused on defining a procedure to produce polycrystalline Ih ice samples, minimizing the presence of defects like air bubbles and cracks - which are known to affect the results of the dielectric measurements. To achieve this purpose, different samples were prepared using different sample holders and cooling rates and then analysed qualitatively and quantitatively using microtomography. Once the most reliable procedure to minimize ice defects was assessed, samples of pure ice were produced in a climatic chamber simultaneously using the microtomography and the dielectric cells, to test the possibility to perform structural analysis and dielectric measurements on the same type of ice. Dielectric measurements were performed using both a capacitive cell connected to an LCR-meter instrument and a coaxial line connected to a VNA. The results of this work confirm that this procedure can be successfully applied to control the integrity of the sample and to assess, at the same time, the dielectric properties of pure Ih ice.

How to cite: Cimbolli Spagnesi, F., Cosciotti, B., Lauro, S. E., Mattei, E., and Pettinelli, E.: Preliminary tests to combine X-ray microtomography and dielectric measurements to assess the radar properties of pure water ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14385, https://doi.org/10.5194/egusphere-egu26-14385, 2026.

EGU26-14842 | ECS | Orals | CR6.3

Dielectric Characterization of Salty-Ice Analogues and Simulations of Radar Signal Propagation Through the Icy Crust of Jovian Moons  

Gabriele Turchetti, Sebastian Lauro, Elena Pettinelli, Barbara Cosciotti, Elisabetta Mattei, and Alessandro Brin
 

The Jovian icy moons – Ganymede, Europa, and Callisto – are of great astrobiological and geophysical interest due to the potential presence of liquid water inside/beneath their icy shells. Among all geophysical methods, Radio Echo Sounding (RES) appears to be the most suitable technique to detect such hidden water, especially as it can operate from an orbiting platform. Starting early 2030s, RIME and REASON, the radar sounders aboard JUICE and Europa Clipper missions, will extensively explore the internal structure of the Galilean moons to search for any evidence of liquid water and to help assessing the habitability conditions of such icy bodies. In order to properly interpret the radar data, the dielectric behaviour of the material composing the crust must be known. Data regarding the dielectric behaviour of salty ices are sparse, especially in the frequency range of such radar sounders, and poorly understood.  

Given the ambiguity in the composition of the icy crusts, a large set of icy analogues should be explored, although laboratory measurements are time consuming and difficult to be properly performed. In this work we start addressing this problem, combining dielectric properties measured in laboratory with radar signal propagation simulations. 

Because the capability of radio waves to investigate deep in the crust depends on signal attenuation that, in turn, is controlled by temperature, type of salt and salt concentration, we performed dielectric measurements at various temperatures and salt concentrations.  We started by considering the most problematic salt, NaCl, as it is known to be able to enter the ice lattice and affect the conductivity of the icy mixture (and thus signal attenuation). We measured the complex dielectric permittivity of NaCl-doped ice samples over a radar frequency range of 1-100 MHz for the salt concentration range 10-1000 mM and the range of temperature 198-292 K, using a two-port Vector Network Analyzer (VNA) coupled with a coaxial cage cell inserted in a climatic chamber. Then, we used the results of such measurements to generate different subsurface scenarios and to run radar simulations at 9 MHz (one of the operational frequencies of RIME and REASON), to assess the detectability of various targets inside the icy crusts and to validate the performance of the radars. 

Our results provide a first hint on the detectability of the water inside/below an NaCl-icy crust and on the penetration depth of the radar signals in different thermal and salt concentration profiles.  

How to cite: Turchetti, G., Lauro, S., Pettinelli, E., Cosciotti, B., Mattei, E., and Brin, A.: Dielectric Characterization of Salty-Ice Analogues and Simulations of Radar Signal Propagation Through the Icy Crust of Jovian Moons , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14842, https://doi.org/10.5194/egusphere-egu26-14842, 2026.

EGU26-14949 * | ECS | Orals | CR6.3 | Highlight

Polarimetric Synthetic Aperture Radar Altimeter (PoSARA): progress towards a new Earth Observation mission concept for snow depth and cryosphere remote sensing 

Rosemary Willatt, Julienne Stroeve, Melody Sandells, Vishnu Nandan, Heather Selley, Anna Hogg, Robbie Mallett, Steve Baker, Amy Macfarlane, Lanqing Huang, Monojit Saha, Alicia Fallows, and Carmen Nab

Sea ice and its snow cover play key roles in Earth's climate. Snow depth and sea ice thickness are World Meteorological Organisation-designated Essential Climate Variables, but their complexity and heterogeneity can pose a challenge for remote sensing. Satellite radar altimetry can provide data over large length and timescales, but there are uncertainties associated with the penetration and scattering of the EM radiation used in these Earth Observation approaches and hence data products. Validation from satellite, airborne and surface-based campaigns do not present a coherent set of results, leading to a lack of clarity on the physics and the way forward for remote sensing approaches. 


The depth of snow on sea ice also remains a major source of uncertainty in sea ice thickness retrievals. Using the KuKa surface based, fully polarimetric dual-frequency radar instrument, deployed in multiple Arctic and Antarctic field campaigns, it has been demonstrated that using dual-polarisation techniques could provide accurate retrievals of snow depth, performing better than dual-frequency Ku- and Ka-band approaches at the surface-based scale, along with coincident sea ice freeboard estimates. We present data over Arctic and Antarctic sea ice, and Arctic tundra, demonstrating the performance of the techniques across these scenarios. Via funding from the European Space Agency's New Earth Observation Mission Ideas (NEOMI) grant, we have developed the concept through scientific readiness levels 1-3. We explore the possibility of scaling to satellite scale and future possibilities for polarimetric altimetry over the cryosphere, using modelling and considerations of upscaling of findings from surface-based campaigns, and contrast our techniques against dual-frequency approaches.

How to cite: Willatt, R., Stroeve, J., Sandells, M., Nandan, V., Selley, H., Hogg, A., Mallett, R., Baker, S., Macfarlane, A., Huang, L., Saha, M., Fallows, A., and Nab, C.: Polarimetric Synthetic Aperture Radar Altimeter (PoSARA): progress towards a new Earth Observation mission concept for snow depth and cryosphere remote sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14949, https://doi.org/10.5194/egusphere-egu26-14949, 2026.

EGU26-16088 | ECS | Orals | CR6.3

Unveiling the Origin and Ice vs Lithic Composition of the Mars North Polar Basal Unit with Multiband Radar Analyses 

Stefano Nerozzi, Michael Christoffersen, and Jack Holt

The basal unit (BU) of Planum Boreum (PB) on Mars is an ice-rich sedimentary deposit between the Late Amazonian North Polar Layered Deposits (NPLD) and the Late Hesperian Vastitas Borealis interior unit. Its two subunits, rupēs and cavi, represent records of polar geologic and climatic processes across most of the Amazonian (~3.3 Ga). The cavi unit likely consists of alternating sand and ice sheet remnants of past polar caps, reflecting volatile–sedimentary interplay, while little is known about rupēs. Thanks to recent advances in radar data processing and dense coverage by the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS), it is now possible to reconstruct the stratigraphy and composition of the BU, and reveal the enigmatic nature of the rupēs unit.

We analyzed over 600 MARSIS profiles at 3, 4, and 5 MHz, leveraging optimized ionospheric corrections and deep penetration to map the full thickness of the BU and retrieve its frequency-dependent complex dielectric permittivity. We find that the rupēs unit spans the western half of PB and part of Olympia Planum as a continuous body beneath the cavi unit with a pole-facing upper unconformity, occupying ~191,000 km³ (~53% of BU volume). Dielectric inversions yield a real permittivity ε’ = 4.0±0.8 (consistent at all frequencies) and a frequency-dependent loss tangent tanδ = 0.017±0.006 (3 MHz) to 0.012±0.006 (5 MHz). Both components of the dielectric permittivity exhibit strong spatial heterogeneity, with values increasing toward Hyperborea Lingula (ε’ > 6, tanδ > 0.02).

These results indicate that the rupēs composition differs substantially from that of the cavi unit, with large loss tangent values indicating the presence of significant amounts of lithic materials despite the low real permittivity. Basalt alteration products with tanδ > 0.02 are required to explain the high loss tangent measurements, while their strong frequency-dependence matches the water ice imaginary permittivity behavior. We find a best match of real dielectric permittivity and loss tangent results using a mixture of 85-90% water ice and 10-15% basalt alteration products like hydrated sulfates (e.g., gypsum), clays, and ferric oxides, which are supported by spectroscopic detections at visible exposures. Rupēs lithic materials may have been transported from lower latitude sources, where aqueous alteration is more viable than at polar latitudes. However, the strong spatial heterogeneities suggest that significant localized alteration occurred in situ during the Amazonian period, perhaps facilitated by warmer high-obliquity periods predicted to occur during the last 3 Gyr. Regardless of their source, the volume of these materials corresponds to a 24 cm–thick global layer, indicating that the rupes unit constitutes a substantial sediment reservoir, not merely one of water ice. Finally, the high loss tangent measured in Hyperborea Lingula explains the lack of rupēs basal detections by SHARAD despite the relatively low thickness (i.e., 150-200 m) of the rupēs unit at that location.

How to cite: Nerozzi, S., Christoffersen, M., and Holt, J.: Unveiling the Origin and Ice vs Lithic Composition of the Mars North Polar Basal Unit with Multiband Radar Analyses, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16088, https://doi.org/10.5194/egusphere-egu26-16088, 2026.

Ice internal thermophysical properties are key factors in the study of dynamics and thermodynamics of ice sheet. Due to the capability of microwave to penetrate ice, several studies have illustrated the feasibility of using active and passive microwave remote sensing approaches to determine the ice internal thermophysical properties, such as temperature profile of ice sheet. On one hand, based on the sensitivity difference across different frequencies to different depth, multifrequency brightness temperature can be used to retrieve ice sheet internal temperature profile. On the other hand, the radar attenuation derived by the ice penetrating radar echo is also strongly correlated with ice temperature. Thus, several studies have tried to develop combined active and passive remote sensing approaches to make better constraints of ice sheet internal temperature profile. In our recent study, a combined active and passive retrieval algorithm for ice sheet internal temperature profile has been developed and demonstrated with ultrawideband radiometer and ice penetrating radar data on Greenland, and an active and passive microwave suite named ICE Penetrating Radar and Thermal Profiler (ICEPATH) including ice penetrating radar and ultrawideband radiometer system is also developed, aiming to detect the internal structure and physical properties of ice sheets and glaciers. This naturally leads us to wonder whether such active and passive microwave remote sensing approaches can be used to make detection of ice shell internal thermophysical properties on icy moons. This study aims to explore the application of active and passive microwave remote sensing approaches on earth polar region in icy moon detection, discussing the mechanism and feasibility of using active and passive microwave remote sensing approaches to detect the ice shell internal thermophysical properties. The results are expected to provide technical basis and serve as important reference for the icy moon exploration missions, supporting the thermal evolution analysis and providing new critical evidences for the existence of subsurface ocean and habitability of icy moon.

How to cite: Bai, D. and Zhu, D.: Active and Passive Microwave Remote Sensing of Ice Internal Thermophysical Properties: from Earth Polar Region to Icy Moon, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16102, https://doi.org/10.5194/egusphere-egu26-16102, 2026.

EGU26-16505 | ECS | Posters on site | CR6.3

Deep-Penetrating UAV-GPR Imaging for Inapparent Landslide Investigation in Rugged Terrain 

Wuji Wang, Tianyang Li, and Nian Yu

An inapparent landslide refers to a subsurface mass movement that develops without producing obvious surface deformation or destruction . Such landslides commonly occur within rock or soil masses that are highly susceptible to fracturing and possess inherently weak internal structures. When triggered by external factors such as rainfall, these concealed landslides can accelerate and expand rapidly, causing abrupt changes in topography and resulting in severe losses of life and property. Crucially, recent studies have identified the bedrock interface as the decisive factor for the stability analysis and early warning of such landslides. However, conventional ground-based monitoring methods provide only sparse point measurements and fail to resolve the continuous subsurface structure.

Unmanned Aerial Vehicle-based Ground-Penetrating Radar (UAV-based GPR) is an efficient and non-destructive geophysical detection technology. It generally consists of the UAV platform, a GPR subsystem, the flight control and basic positioning sensors of the UAV, high-accuracy positioning sensors, and a communications subsystem (Figure 1). Compared to conventional ground-based GPR, UAV-based GPR offers offers a promising non-contact solution for such landslides, enabling rapid and safe surveys over hazardous terrain Nevertheless, in complex mountainous environments, dense vegetation and steep, undulating topography significantly degrade data quality, leading to severe imaging artifacts and interpretation ambiguity .

In this study, we propose reverse time migration (RTM) formulated in a curvilinear coordinate system for UAV-based GPR. Subsequently, we introduce an interface extraction technique to accurately identify the continuous bedrock interface from the migration profiles. For data acquisition, we deploy a low-frequency UAV-based Stepped‑Frequency Continuous‑Wave GPR (SFCW-GPR) system in the landslide-prone regions of Sichuan Province. The system achieves effective penetration depths of up to 20 m while maintaining stable imaging quality. These results indicate that the proposed framework provides a practical and high-resolution solution for the identification and structural characterization of inapparent landslides in complex mountainous environments.

Figure 1 The UAV-based GPR system used for landslide investigation.

How to cite: Wang, W., Li, T., and Yu, N.: Deep-Penetrating UAV-GPR Imaging for Inapparent Landslide Investigation in Rugged Terrain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16505, https://doi.org/10.5194/egusphere-egu26-16505, 2026.

EGU26-17069 | Posters on site | CR6.3

Performance assessment of JuRa internal structure imaging of Didymos using gradient descent algorithms with a linearized forward operator 

Yann Berquin, Alain Hérique, Yves Rogez, Wlodek Kofman, and Sonia Zine

This study details preliminary work for the data processing of JuRa spaceborne planetary sounding radar which will investigate the interior of the binary S-type asteroid Didymos in 2027 as part of the ESA Hera mission [1]. Spaceborne planetary sounding radars are designed to remotely probe planetary bodies subsurface at decametric to metric resolutions at depths ranging from few hundred meters up to few kilometers depending on the carrier frequency used. These radar characteristics are driven by geophysical (e.g. penetration and spatial resolution) and technical considerations (e.g. power and antenna size). JuRa was designed as a monostatic radar with an antenna composed of two crossed 1.5m dipoles able to emit Binary Phase Shift Keying (BPSK) coded signals in a 20 MHz bandwidth centered around a 60 MHz carrier, and 5 W peak power. Such configuration allows to emit and receive with either dipole antennas allowing full polarization characterization. In order to perform 3D internal structure imaging, a sufficient diversity of geometry of acquisition is required involving multiple orbits and sounding measurements on each orbit. One of the major challenge when exploiting radar data data to reconstruct the internal structure of kilometric-size planetary bodies lies in the relatively large size of the planetary body with regard to the radar carrier signal wavelength. Accordingly, processing JuRa downlinked data using Full Waveform Inversion (FWI) to reconstruct the internal structure of Didymos (800m diameter) and its moon Dimorphos (160m diameter) will prove a computationally challenging task given the relatively short radar carrier signal wavelength (~5m). In order to overcome this limitation, we investigate the possibility to use gradient descent algorithms with a linearized forward operator to process data from spaceborne planetary sounding radar dedicated to asteroid interior imaging. Performances of the proposed internal structure imaging algorithm are evaluated on a previously published asteroid analog anechoic chamber dataset [2] using Discrete Dipole Approximation to compute electric fields. Results showcase the ability to recover main interior structures in the analog case opening promising perspectives for JuRa data processing and for future asteroid interior sounding radars.

[1] P. Michel, M. Küppers, A. C. Bagatin, B. Carry, S. Charnoz, J. De Leon, A. Fitzsimmons, P. Gordo, S. F. Green, A. Hérique, et al., “The esa Hera mission: detailed characterization of the Dart impact outcome and of the binary asteroid (65803) Didymos,” The planetary science journal, vol. 3, no. 7, p. 160, 2022.

[2] A. Dufaure, C. Eyraud, L.-I. Sorsa, Y. Yusuf, S. Pursiainen, and J.-M. Geffrin, “Imaging of the internal structure of an asteroid analogue from quasi-monostatic microwave measurement data – I. the frequency domain approach,” Astronomy & Astrophysics, vol. 674, p. A72, 2023.

How to cite: Berquin, Y., Hérique, A., Rogez, Y., Kofman, W., and Zine, S.: Performance assessment of JuRa internal structure imaging of Didymos using gradient descent algorithms with a linearized forward operator, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17069, https://doi.org/10.5194/egusphere-egu26-17069, 2026.

EGU26-18760 | Posters on site | CR6.3

Cryo-TEMPO: a CryoSat-2 Thematic Product over Land Ice 

Malcolm McMillan, Karla Boxall, Alan Muir, Alessandro Di Bella, Michele Scagliola, and Jérôme Bouffard

Since its launch in 2010, CryoSat-2 has continued the long-term radar altimeter record, and provided over a decade of measurements with which to monitor and understand the polar ice sheets. Although these datasets have historically been distributed by ESA as Level-2 products, following consultations with the wider glaciological community, it has become increasingly clear that there is significant untapped value that can be realised by expanding the user-base through the development of a dedicated L2 Thematic Land Ice Product. Crucially, this requires simplified, agile and state-of-the-art products and processing flows, which are updated regularly, and deliver an easy-to-use dataset whilst maintaining the native along-track sampling of the original Level-2 products. Thus, ESA has embarked on a new path towards developing CryoSat-2 Thematic Products, which aim to drive further innovation and exploitation, and have created a model that has now been replicated across other radar altimeter missions.

Here, we present the latest Cryo-TEMPO Land Ice product. The over-arching objectives of Cryo-TEMPO are (1) to implement dedicated, state-of-the-art processing algorithms, (2) to develop agile, adaptable processing workflows, that are capable of rapid evolution and processing at high cadence, (3) to create products that are driven by, and aligned with, user needs; thereby opening up the data to new communities of non-altimetry experts, and (4) to deliver transparent and traceable uncertainties. We provide an overview of the Land Ice product, a review of the current generation of this thematic product, and look ahead to the evolutions planned for the next phase of the study.

How to cite: McMillan, M., Boxall, K., Muir, A., Di Bella, A., Scagliola, M., and Bouffard, J.: Cryo-TEMPO: a CryoSat-2 Thematic Product over Land Ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18760, https://doi.org/10.5194/egusphere-egu26-18760, 2026.

EGU26-20497 | Posters on site | CR6.3

Quantifying runoff in Greenland’s percolation zone with phase-sensitive radar and firn modeling 

Falk M. Oraschewski, Baptiste Vandecrux, Anna Puggaard, Reinhard Drews, Nanna B. Karlsson, Keith W. Nicholls, Andreas P. Ahlstrøm, Andrew Tedstone, Horst Machguth, and Anja Rutishauser

Surface melting and runoff account for about half of the current mass loss of the Greenland Ice Sheet. Regional climate models (RCMs) project runoff to increase further over the 21st century, but the magnitude of this trend varies strongly between different models. This variability arises because RCMs rely on simplified representations of the complex firn hydrological system in Greenland’s percolation zone. However, key parameters for parametrizing meltwater retention and runoff processes remain poorly constrained due to a lack of time-resolved, in situ observations of firn liquid water content.

We address this gap by demonstrating that the Autonomous phase-sensitive Radio-Echo Sounder (ApRES) can continuously trace the amount of liquid water in the firn. At three automatic weather station sites on the ice sheet (KAN_U, DYE-2 and Camp Century), we acquired hourly ApRES time series between spring 2023 and 2025, covering two melt seasons. By analyzing these observations in combination with a firn model, we quantify rates of lateral meltwater flow. Comparison with runoff simulations from three RCMs shows that all models overestimate local runoff at KAN_U, and that some even predict runoff at DYE-2 (2124 m a.s.l.), where our observations indicate that all meltwater is refrozen. Expanding these observations will support the development of improved representations of Greenland’s firn hydrological system in RCMs and ultimately enhance the accuracy of GrIS mass balance projections.

How to cite: Oraschewski, F. M., Vandecrux, B., Puggaard, A., Drews, R., Karlsson, N. B., Nicholls, K. W., Ahlstrøm, A. P., Tedstone, A., Machguth, H., and Rutishauser, A.: Quantifying runoff in Greenland’s percolation zone with phase-sensitive radar and firn modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20497, https://doi.org/10.5194/egusphere-egu26-20497, 2026.

Changing climate conditions are causing significant impacts for Arctic communities and the landscapes, ecosystems and infrastructure they rely on. Rapid permafrost degradation is not uniform over space or time and there are a variety of variables contributing to the vulnerability of different infrastructure to thaw-related hazards. These include event-based changes such as heat waves, rainfall, and storm surge events, and longer term shifts such as rising sea levels, groundwater processes during thaw season, and heat transfer from construction materials. The relative influences and interactions between these controls on the rate and nature of permafrost degradation remain poorly understood.

This work leverages correlated Ground Penetrating Radar (GPR) validated with ground probing to examine the spatial changes of the depth to base of the active layer. The GPR data have been characterised into different landscape types; those with a sand/sea interface, untouched tundra, road construction, airport aprons, and made (constructed) ground. The use of GPR prevents destruction and disruption to the already vulnerable permafrost and provides continuous subsurface mapping data. Simplified 2D numerical models have been created using electromagnetic simulation software (gprMax) to parameterise the findings from the measured field data. The purpose of this is to verify the assumptions of the processed GPR data, without the need for destructive borehole testing or coring, as would have been used historically. The combination of modelling and survey data shows the impact of the different landcover types on permafrost degradation and provides the community with valuable knowledge on the impacts of distinct alterations in land use on permafrost, allowing more informed decisions on best building practices.

These findings demonstrate the impact of assumptions made in the field of GPR settings and highlight its effectiveness in detecting the permafrost to active layer interface under different conditions. When combined with the 2D model interpretations GPR surveys offers a targeted training dataset that can potentially be scaled with earth observation data, targeting specific features, settings and infrastructure that impact permafrost degradation.

How to cite: Coote, G., Warren, C., Lim, M., Lee, R., Martin, J., and Whalen, D.: Characterising the spatial variability of permafrost measurements in different landscape types at the climate impacted coastal communities in the Inuvialuit Settlement Region, Canada, using Ground Penetrating Radar , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22545, https://doi.org/10.5194/egusphere-egu26-22545, 2026.

EGU26-308 | ECS | Orals | CR6.5

Daily Cloud-Free NDSI Reconstruction Across the Northern Hemisphere Driven by Nonlinear Meteorological Forcing 

Jiahui Xu, Yan Huang, Stef Lhermitte, Ruiyang Hua, and Bailang Yu

Persistent cloud contamination in MODIS normalized difference snow index (NDSI) products severely limits reliable snow cover monitoring across the Northern Hemisphere, making effective gap-filling crucial. However, existing approaches often oversimplify snow temporal dynamics and fail to capture the cumulative nature of snow–climate interactions. To address these limitations, we propose PredFormer, a novel sequence-based framework that extends the self-attention mechanism to the temporal dimension, thereby explicitly modeling the nonlinear temporal evolution of NDSI coupled with cumulative meteorological effects. The framework further incorporates vegetation growth, topographic conditions, and cloud mask information to account for complex environmental dependencies. Validation results demonstrate that PredFormer achieves superior reconstruction performance across the Northern Hemisphere, with MAE and RMSE values of 1.110 and 2.946, respectively. Notably, the distinct mechanism of incorporating nonlinear cumulative meteorological effects reduces RMSE by 11.57%, and comparative analyses against baseline models (e.g., LSTM and standard Transformers) reveal performance gains exceeding 19%. The framework also demonstrates substantial improvements in high-elevation and forested regions—including the Hindukush–Himalaya and the West Coast. Leveraging this framework, we generate the first hemispheric-scale, daily cloud-free NDSI dataset (5-km resolution, 2003–2023). This work not only advances the methodological handling of nonlinear snow dynamics but also delivers a foundational dataset for hydrological modeling and climate change assessment.

How to cite: Xu, J., Huang, Y., Lhermitte, S., Hua, R., and Yu, B.: Daily Cloud-Free NDSI Reconstruction Across the Northern Hemisphere Driven by Nonlinear Meteorological Forcing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-308, https://doi.org/10.5194/egusphere-egu26-308, 2026.

EGU26-347 | Orals | CR6.5

snowMapper v1.0: a model for daily mountain snow cover reconstruction in high resolution 

Konstantis Alexopoulos, Ian C. Willis, Hamish D. Pritchard, Giorgos Kyros, Vassiliki Kotroni, and Konstantinos Lagouvardos

snowMapper is a physics-informed model developed to generate daily reconstructions of snow cover across complex mountain terrain. The system integrates in situ measurements with gridded meteorological inputs and incorporates binary snow presence/absence observations derived from high-resolution satellite imagery. Its modular design enables users to tailor configurations to specific study sites, producing daily snow-cover maps at spatial resolutions typically ranging from 20 to 100 meters. The workflow includes a preprocessing pipeline compatible with imagery from Landsat 4–9 and Sentinel-2; multiple terrain- and land-cover–based masking options (i.e., forest, glaciers, surface water, elevation, urban areas); five configurable schemes for converting satellite reflectance to binary snow cover; and a quasi–physically based downscaling of climate variables. Snow-cover reconstruction is accomplished through two sequential, configurable gap-filling procedures: an initial decision-tree step followed by a machine-learning classifier. The classifier can be trained either with local field observations or with in situ data originating from other regions, allowing the model to operate in a fully physics-informed mode in the absence of a local monitoring network. A built-in evaluation module compares model outputs with satellite-derived snow cover, providing accuracy metrics directly within the final product. Optional aggregation routines allow fractional snow-cover metrics to be generated across temporal and spatial scales. The system operates entirely on Google Earth Engine via its Python API, reducing dependence on local data storage and eliminating local computational demands. We applied snowMapper to generate a 41-year snow-cover climatology for Greek mountains exceeding 2,000 m a.s.l. The resulting daily 100 m climatology consisted of over 90 % modeled values, and achieved a mean overall accuracy of 93 % when assessed against 1.1 billion clear-sky, pixel-level satellite observations. The model code and example data are available as an open-source project on GitHub (https://github.com/snowMapper/snowMapper, last access: 25 November 2025).

How to cite: Alexopoulos, K., Willis, I. C., Pritchard, H. D., Kyros, G., Kotroni, V., and Lagouvardos, K.: snowMapper v1.0: a model for daily mountain snow cover reconstruction in high resolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-347, https://doi.org/10.5194/egusphere-egu26-347, 2026.

Current GLOF (Glacial Lake Outburst Floods) risk assessments in High Mountain Asia (HMA) are often limited by static glacial lake inventories and unreliable Area-Volume (A-V) scaling models, which are not widely validated in the region. In this study, we developed a fully automated framework integrating multi-source remote sensing (e.g. Landsat, Sentinel-1/2, Copernicus DEM) and satellite altimetry (ICESat-2) to monitor glacial lake dynamics. We map nearly 32,000 glacial lakes across HMA for 2022 with a detection accuracy of 96% and relative boundary accuracy of 98% for lakes >20,000 m², offering a significant improvement over manual inventories. Our analysis shows three important results. First, regional heterogeneity is pronounced across the HMA sub-regions. For instance, East Kun Lun exhibited the highest expansion rate (8% area increase, 2016–2022), highlighting the need for targeted hazard assessment, while West Himalaya showed minor change (0.04%). Second, by processing ICESat-2 data for >16,000 lakes, we validated widely used A-V scaling models. Our results demonstrate that large supraglacial and extra-glacial lakes exhibit volume estimation errors exceeding 1500% in standard models, highlighting a significant bias in current flood volume potential estimates. Third, our automated temporal monitoring identified four GLOF events during the study period that were not previously documented. Analysis of these events reveals distinct area peaks before GLOFs, providing quantifiable indicators for early warning. This framework utilizes open-source remote sensing data on the Google Earth Engine cloud platform for regular monitoring of glacial lakes with higher accuracy while providing a reproducible, scalable method to correct volume estimates and detect hidden GLOF events in high-mountain valleys.

How to cite: Kumar, R. and Vijay, S.: Automated Multi-Sensor Framework for Glacial Lake Dynamics and Unreported GLOF Detection across High Mountain Asia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-702, https://doi.org/10.5194/egusphere-egu26-702, 2026.

EGU26-744 | ECS | Posters on site | CR6.5

Automated Mapping of Glacier Frontal Retreat in the Indian Himalaya using Satellite Remote Sensing and Deep Learning models 

Sarvesh kumar Verma, Saurabh Vijay, and Argha Banerjee

The Himalayan glaciers continue to lose mass due to the undergoing warming climate. They play a critical role in feeding major rivers, such as the Ganga, Indus, and Brahmaputra, supporting the livelihoods of millions. While regional mass changes have been reported by several studies, the current retreat rates are rarely documented. This is primarily due to a lack of satellite data and methods in mapping debris-covered glacier fronts. They are also limited in distinguishing clean ice and perennial snow cover patches. While the global glacier database, such as the RGI (Randolph Glacier Inventory), provides a critical database, it is based on satellite images from 2000-2003.  

In this study, we address challenges in mapping debris-covered glaciers by combining Deep Learning (DL) and a geometric algorithm. We apply several DL models (e.g., including UNet++, GlacierNet-2, GlaViTU, M-LandsNet, and SAU-Net) on multiple remote sensing satellite datasets, which include spectral, radar, topography, geomorphology, and glaciological dynamics. The study sites include four basins of the Himalaya (Chandra Bhaga, Pangong, Chombu Chu, and Alaknanda-Bhagirathi). UNet++ shows the most accurate results with reference outlines, with a mean Intersection over Union (IoU) of ~ 90%. DL-based retreat measurements were closely aligned with those outlined in the reference manual, with a coefficient of determination (R²) of ~ 75%. Our applied Python-based geometric algorithm calculates the average euclidean distance between frontal positions in 2010 and 2019. We find that the retreat rates of debris-covered glaciers in these basins are ~3 m/year during this period.  Lake-terminating glaciers show three times higher retreat rates in the period. This algorithm has the capability to detect glaciers of all sizes, ranging from small to large glaciers, as well as highly debris-covered to clean-ice glaciers, and can identify cirques to hanging glaciers in all the basins.

This DL-based algorithm provides an automated approach with post-processing steps to monitor glacier change with high precision, accounting for the uncertainty of glacier retreat across the Himalaya. This study is important for understanding the relationship between glacier lake expansion and glacier ice mass loss, which can be further used for glacier hazards, such as lake outbursts and dry calving detachments.

How to cite: Verma, S. K., Vijay, S., and Banerjee, A.: Automated Mapping of Glacier Frontal Retreat in the Indian Himalaya using Satellite Remote Sensing and Deep Learning models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-744, https://doi.org/10.5194/egusphere-egu26-744, 2026.

Seasonal variability in the ice velocities of slow-moving Himalayan glaciers (≤100 m yr⁻¹; >4000 m a.s.l.) is largely unknown, primarily due to the scarcity of high-resolution observations and the substantial uncertainties associated with satellite-based velocity products. In this study, we present high-frequency terrestrial time-lapse camera (TLC) observations of glacier ice motion from Drang Drung Glacier (33.76° N, 76.30° E), spanning October 2023 to April 2025. The glacier terminus is predominantly lake-terminating, with a smaller land-terminating component, enabling a comparative assessment of spatial variations in ice dynamics.

Our results show spatial heterogeneity in surface velocity. Annual mean velocities at the lake-terminating section (35.4 m yr⁻¹) are nearly twice those observed at the adjacent land-terminating segment (19.5 m yr⁻¹). A primary seasonal cycle is evident in both regions, characterised by summer speedup (June–September) followed by autumn slowdown (September–November). These variations correspond closely with increases in air temperature and solar radiation, and are consistent with the meltwater-driven evolution of the subglacial drainage system from inefficient to efficient, channelised configurations. TLC imagery further captures signatures of active subglacial hydrology and its temporal transitions.

A secondary, modest winter speedup (November–January), followed by persistent deceleration until February, suggests that viscous deformation and associated closure of subglacial channels lead to elevated basal water pressures from trapped meltwater. Vertical ice displacement exhibits substantial seasonal variability (−0.9 to −2.0 m month⁻¹) from June to October, with minimal changes outside this period. Sub-weekly analyses reveal coherent patterns of glacier acceleration, contemporaneous increases in lake turbidity, and uplift of the ice front, indicating rapid responses to fluctuations in basal water pressure. TLC-derived velocities show strong agreement with in-situ GNSS measurements but highlight a marked underestimation of glacier motion in ITS_LIVE satellite products for this site.

How to cite: Singh, P. and Vijay, S.: Seasonal ice velocity of Drang Drung Glacier, in the western Himalaya, using terrestrial time-lapse camera imaging , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-961, https://doi.org/10.5194/egusphere-egu26-961, 2026.

EGU26-1572 | Posters on site | CR6.5

High resolution monitoring of Greenlandic ice marginal lakes 

David Rippin, Pete Tuckett, Duncan Quincey, Connie Harpur, Alex Scoffield, Josh Abraham, Lauren Rawlins, Joe Mallalieu, Hannah Barnett, Jenna Sutherland, Iestyn Woolway, Chris Merchant, Niall McCarroll, Laura Carrea, and Weijia Wang

At present, 10% of the Greenland Ice Sheet (GrIS) margin terminates in a lake, but this is forecast to increase significantly over coming decades with ongoing retreat and thinning of the ice margin. This is important because the existence of more and larger lakes implies greater mass loss at the margin as well as an increase in dynamic thinning up-ice. At the same time, non-glacial lake surface waters worldwide have been shown to be warming yet the record of temperature change in ice-marginal lakes is extremely sparse. These ice-marginal lakes are likely to become increasingly important drivers of mass loss, and so there is an urgent need to investigate more closely the connection between their evolution and changes in the ice sheet. Therefore, a key objective is to explore the thermal properties of these lakes.

The majority of Greenland’s ice marginal lakes are small (<0.5km2) thus limiting the role of remote sensing approaches. To fully characterise and understand the detailed thermal properties of these lakes over time and space we thus developed an in-situ approach for high resolution monitoring of the temperature evolution of two Greenlandic ice marginal lakes. Our monitoring approach involved the installation of a series of thermistor strings which recorded water temperature at several locations and at a range of depths every 30 minutes for more than one year. Over the same period we deployed a series of 15 time-lapse cameras capturing hourly imagery so as to build 3D models of ice front change in response to changing lake properties. Finally, we carried out several drone-based surveys using a thermal camera to record spatially distributed lake temperatures. As well as discussing our monitoring network, we also present data that reveals Greenlandic lake evolution at a resolution not previously seen, showcasing an observational framework that could be replicated at other lake-terminating sites elsewhere in the world. 

How to cite: Rippin, D., Tuckett, P., Quincey, D., Harpur, C., Scoffield, A., Abraham, J., Rawlins, L., Mallalieu, J., Barnett, H., Sutherland, J., Woolway, I., Merchant, C., McCarroll, N., Carrea, L., and Wang, W.: High resolution monitoring of Greenlandic ice marginal lakes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1572, https://doi.org/10.5194/egusphere-egu26-1572, 2026.

EGU26-5118 | ECS | Orals | CR6.5

Deep-learning-based mapping reveals multi-decadal crevasse evolution on Antarctic ice shelves from Landsat imagery 

Leyue Tang, Jonathan Louis Bamber, and Gang Qiao

Antarctic ice shelves buttress grounded ice and play a critical role in regulating glacier stability and the mass balance of the Antarctic Ice Sheet. Over recent decades, many Antarctic ice shelves have exhibited significant mass loss. Crevasses, which formed in response to internal stresses, are key indicators of ice shelf stability and their development is intricately coupled to the evolving ice dynamics. However, consistent long-term and high-resolution records of crevasse evolution over Antarctic ice shelves remain limited.

Here, we present a continuous and automated mapping of crevasses on representative Antarctic ice shelves from 1999 to 2024 using Landsat 7 and Landsat 8 imagery and a deep-learning-based segmentation framework at 30 m resolution. A manually delineated dataset based on Landsat 8 RGB imagery from multiple ice shelves, encompassing a wide range of crevasse morphologies, was constructed for model training and validation. To address the scan-line corrector (SLC) failure of Landsat 7 ETM+ since 2003, we developed a diffusion-based gap-filling approach trained on a dataset specifically constructed for this study, enabling consistent crevasse mapping across the full Landsat 7/8 archive.

Our results reveal pronounced crevasse development on Pine Island, Thwaites, and Larsen B Ice Shelves over the past two decades, while other mapped ice shelves exhibit more moderate or minimal changes. This long-term, high-resolution crevasse mapping provides new insights into ice shelf damage evolution and offers valuable constraints for damage parameterization and assessments of ice shelf stability. The developed pipeline is readily extendable to additional ice shelves and remains computationally efficient.

How to cite: Tang, L., Bamber, J. L., and Qiao, G.: Deep-learning-based mapping reveals multi-decadal crevasse evolution on Antarctic ice shelves from Landsat imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5118, https://doi.org/10.5194/egusphere-egu26-5118, 2026.

The growth of ice slabs influences both the spatial extent and the rate at which the Greenland Ice Sheet’s wet snow zone transitions from storing meltwater in firn, to exporting it as surface runoff. These changes reorganize meltwater storage and flow pathways, shaping the ice sheet’s contribution to sea level rise. In this work, we combine Sentinel-1 (S1) C-band satellite radar mosaics with Operation IceBridge (OIB) airborne radar profiles to produce a decade long time series of ice slab expansion in Greenland. To efficiently process the large S1 data volume, we use Google Earth Engine to compile Interferometric Wide and Extra Wide Swath data acquired during boreal winters (1 November – 30 March) from 2015 to 2025, producing annual co-polarized (HH) and cross-polarized (HV) backscatter mosaics that are multilooked and linearly corrected to a common incidence angle. We then use logistic regression to optimize ice slab detection thresholds and to quantify classification uncertainty.

Our time series reveals pronounced differences in the rate of ice slab expansion between northern and southwest Greenland. Isolated OIB radargrams also suggest marked differences in ice slab geometry between these two regions. In northern Greenland, thick downflow ice slabs transition abruptly into laterally extensive, thin ice slabs that extend tens of kilometers upslope into the percolation zone. In contrast, ice slabs in southwest Greenland either remain thick at their upflow fronts or, when thin, occur deeper in the firn column and are rapidly buried by subsequent accumulation events. To capture these contrasting ice slab front geometries, we develop a refined classification scheme to map thick and thin ice slabs across the Greenland Ice Sheet using Sentinel-1 backscatter thresholds. The observed spatial and temporal patterns point to regions where atmospheric forcings and percolation zone firn conditions have restricted meltwater infiltration depth, accelerating shallow ice slab growth and altering the near-surface hydrologic regime.

How to cite: Mutter, E. and Culberg, R.: Sentinel-1 based time series of ice slab extent reveals regional divergence in ice slab evolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6029, https://doi.org/10.5194/egusphere-egu26-6029, 2026.

EGU26-6153 | ECS | Orals | CR6.5

Greenland wintertime buried lake drainage and ice dynamics response 

Jianing Wei, Kang Yang, Yuxin Zhu, Yuhan Wang, and Xiaoyu Guo

Buried lakes are widely distributed on the Greenland Ice Sheet (GrIS) after summer. Some of these lakes may drain over winter, thereby delivering meltwater into the ice sheet and potentially influencing ice flow dynamics. However, to date, only a limited number of buried lake drainages (BLDs) have been identified and their spatiotemporal dynamics across the GrIS remain unclear. Here we first detect pan-GrIS wintertime BLDs by integrating Sentinel-1 and -2 satellite imagery and ArcticDEM data, and then investigate potential ice velocity anomalies (IVAs) triggered by BLDs using ice velocity data. The results show that a total of 167 complete and partial BLDs are identified over seven winters from 2017 to 2023 on the GrIS, including 25 cascade drainages. Ten significant IVAs are observed in association with BLDs, and they may lead to net increases in annual ice motion. A representative cascade drainage further reveals that partial BLDs may result from the combined effects of the fracture location and depression topography. Meanwhile, the depression topography and associated water storage capacity may be markedly altered by wintertime drainage. Notably, beyond triggering IVAs of up to ~50%, some BLDs can even trigger rerouting of subglacial hydrologic pathways within a few days.

How to cite: Wei, J., Yang, K., Zhu, Y., Wang, Y., and Guo, X.: Greenland wintertime buried lake drainage and ice dynamics response, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6153, https://doi.org/10.5194/egusphere-egu26-6153, 2026.

EGU26-6817 | ECS | Posters on site | CR6.5

U-DEM: High spatiotemporal resolution surface elevations of the Canadian Arctic 

Ann-Sofie Priergaard Zinck, Jonathan Ortved Melcher, and Dorthe Dahl-Jensen

Monitoring glacier surface elevation - and thus thickness - changes at high spatiotemporal resolution is essential for improving projections of future mass loss, constraining ice-flow models, and understanding the processes driving observed variability. Here, we present U-DEM, a new ice surface elevation dataset for the Canadian Arctic at 100 m spatial and 3-monthly temporal resolution, spanning the period from the launch of Sentinel-1 in 2014 through 2024. The dataset is generated using a deep-learning framework that combines CryoSat-2 swath altimetry, Sentinel-1 SAR imagery, and ArcticDEM stereo-derived elevation strips to produce a continuous, high-resolution record of surface elevation change.

First results demonstrate that the approach successfully captures spatial and temporal variability in glacier surface elevations that is not resolved by CryoSat-2 alone. The resulting DEMs show a substantially lower root-mean-squared-error than CryoSat-2, while reproducing small-scale topographic features such as narrow outlet glaciers and complex marginal zones. These improvements are particularly important in regions characterized by steep gradients and dynamic glacier behaviour.

By providing a consistent, high-resolution elevation time series across the Canadian Arctic, U-DEM opens new possibilities for a wide range of glaciological applications. These include transient modelling of glacier evolution, inverse modelling to constrain bedrock topography, particularly in regions affected by surging glaciers, and investigations of seasonal variability and the processes driving surface elevation changes. Beyond the Canadian Arctic, the U-DEM framework is designed to be transferable and can, in principle, be applied to any region of interest where Sentinel-1 and CryoSat-2 data are available.

How to cite: Zinck, A.-S. P., Melcher, J. O., and Dahl-Jensen, D.: U-DEM: High spatiotemporal resolution surface elevations of the Canadian Arctic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6817, https://doi.org/10.5194/egusphere-egu26-6817, 2026.

EGU26-6902 | Posters on site | CR6.5

The retrieval of the liquid water content in snow from solar light spectral reflectance measurements 

Alexander Kokhanovsky, Karl Segl, Biagio DI Mauro, Claudia Ravasio, Roberto Colombo, and Jörg Bendix

It is known for a long time that the solar light reflectance around 1030nm ice absorption band is sensitive to the liquid water content (LWC) in snow [1]. In particular, this feature has been used to derive the abundance of water in melting snow using an imaging spectrometer [2]. In this work we propose a new technique to derive the snow LWC measuring snow reflectance at three wavelengths (1000, 1020, and 1060nm) together with independent measurements of snow density. The spectral measurements are used to derive the relative snow LWC defined as the ratio of volumetric concentration of water to that of ice in melting snow. The independently measured snow density is needed for the calculation of the snow liquid water content. The developed retrieval technique is fast, simple and can be easily implemented for the express analysis of the snow LWC distribution in the field. The theoretical model is based on the assumption that wet snow can be presented as a collection of air pockets in ice-water matrix [3]. The technique is validated using independent LWC measurements over melted snow performed in combination with snow density and snow hyperspectral reflectance measurements in Italian Alps [4]. The close correspondence of the measured and retrieved LWC in the range 8 - 18% is found.

References

[1] R. O. Green, J. Dozier,  D. Roberts, T. Painter, ''Spectral snow - reflectance models for grain size and liquid water fraction in melting snow for the solar-reflected spectrum'', Ann. Glaciol., vol. 34, pp. 71–73, 2002, https://doi.org/10.3189/172756402781817987.

[2] R. O. Green, T. H. Painter, D. A. Roberts, J. Dozier, ''Measuring the expressed abundance of the three phases of water with an imaging spectrometer over melting snow'', Water Resour. Res., vol. 42, W10402, 2006,  doi:10.1029/2005WR004509.

[3] A. A. Kokhanovsky, K. Segl, J. Bendix, ''Reflectance of solar light from wet snowpack: direct and inverse problems'', IEEE Trans. Geosci. Remote Sens.., 2026,  doi: https://ieeexplore.ieee.org/document/11322691.

[4] C. Ravasio, R.  Garzonio, B. Di Mauro, E.  Matta, C.  Giardino, M. Pepe, et al. , ''Retrieval  of snow liquid water content from radiative transfer model, field data and PRISMA satellite  data'', Remote Sens. Env., vol. 311, 2024, 10.1016/j.rse.2024.114268.

How to cite: Kokhanovsky, A., Segl, K., DI Mauro, B., Ravasio, C., Colombo, R., and Bendix, J.: The retrieval of the liquid water content in snow from solar light spectral reflectance measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6902, https://doi.org/10.5194/egusphere-egu26-6902, 2026.

EGU26-7471 | ECS | Posters on site | CR6.5

Multi-sensor satellite-based vegetation mapping in the Antarctic Peninsula through machine learning 

Miguel Correia and Pedro Pina

The ice-free areas of the Antarctic Peninsula are undergoing significant ecological changes due to regional warming, leading to the expansion of opportunistic vegetation, primarily mosses and lichens. Mapping these communities is essential for long-term ecological monitoring, yet it remains a challenge due to the high spatial fragmentation and spectral similarity of the land cover types.

This study evaluates the effectiveness of different satellite sensors and machine learning algorithms for automated vegetation classification in the ice-free areas of Barton Peninsula (King George Island). Using high-resolution WorldView-2 (2020) and medium-resolution Sentinel-2 and Landsat 8 (2023) imagery, we compared the performance of Support Vector Machines (SVM), Random Trees (RT), and k-Nearest Neighbours (kNN) classifiers through both pixel-based and object-based approaches.

Results indicate that the kNN classifier achieved the highest overall accuracy (OA = 0.91; Kappa = 0.87) when applied to WorldView-2 data, outperforming the traditionally favoured SVM in this specific environment. The study also highlights the limitations of coarser resolution sensors (Sentinel-2 and Landsat 8) in capturing small, fragmented patches of vegetation, where the "mixed pixel" effect remains a significant hurdle, assessing how the results can still be considered meaningful.

The developed methodology demonstrates that multi-sensor remote sensing is a robust tool for creating baseline vegetation maps. These maps are crucial for quantifying the "greening" of Antarctica and provide a scalable framework for environmental conservation efforts under the Antarctic Treaty System.

How to cite: Correia, M. and Pina, P.: Multi-sensor satellite-based vegetation mapping in the Antarctic Peninsula through machine learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7471, https://doi.org/10.5194/egusphere-egu26-7471, 2026.

EGU26-8399 | ECS | Orals | CR6.5

High-Resolution Snowpack Monitoring from a Multi-Sensing Gondola  

Mathieu Le Breton and Alec van Herwijnen

Many snow processes operate at the slope scale and sub-daily timescales, yet observations at these scales remain scarce. We demonstrate a mobile, automated monitoring approach that captures snowpack evolution in mass, thermal state, and liquid water content at the slope scale and sub-daily resolution.

The system combines lidar and photogrammetry with a new RFID-based microwave method, which uses a cable car to repeatedly observe an entire slope. The RFID approach relies on passive tags installed on the ground and covered by snow. When the cable car passes above them, a mobile reader interrogates them at 865–868 MHz, and they respond using backscattering communication. The variation in the signal's phase and signal strength over time is used to monitor snow water equivalent and liquid water content. In parallel, lidar and photogrammetry resolve snow depth and microtopography, while temperature sensors embedded in the tags measure basal snow temperature.

The approach was first implemented on the Pischa slope near Davos, Switzerland. During the 2024–2025 winter, more than 1,000 runs were completed along a 2 km transect spanning 700 m of elevation, and a second campaign is ongoing in the 2025–2026 winter.

The resulting dataset, unique in its spatiotemporal resolution, opens new possibilities to observe rapid snow processes at the slope scale.

Related references:

  • Le Breton, Mathieu et van Herwijnen, Alec. 2025. « High-Resolution Aerial Snowpack Monitoring via Passive RFID (GONDO-RFID) ». P. 1‑6 in 2025 IEEE International Conference on RFID Technology and Applications (RFID-TA).
  • Charléty, Arthur, Mathieu Le Breton, Morgane Magnier, Éric Larose, Laurent Baillet, Ludovic Moreau, et Alec van Herwijnen. 2025. « Locating RFID Tags Under Snow and Vegetation ». P. 1‑5 in 2025 IEEE International Conference on RFID Technology and Applications (RFID-TA).

How to cite: Le Breton, M. and van Herwijnen, A.: High-Resolution Snowpack Monitoring from a Multi-Sensing Gondola , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8399, https://doi.org/10.5194/egusphere-egu26-8399, 2026.

EGU26-8407 | ECS | Posters on site | CR6.5

Identifying Snow Surface Controls on UAV Lidar Intensity for Grain Size Retrieval 

Chelsea Ackroyd and Matt Olson

Beyond lidar’s established role in snow hydrology for mapping snow depth, lidar intensity measurements offer a promising means of informing surface energy balance through retrieval of snow grain size, a primary control on snow albedo and net shortwave radiation. In particular, near-infrared aerial lidar intensity has demonstrated strong potential for retrieving snow reflectance and grain size over mountainous watersheds when corrections for range and incidence angle are applied. However, the accuracy of lidar intensity correction (and subsequent grain size retrieval) is highly sensitive to the quality of calibration data, which has typically relied on coincident imaging spectroscopy reflectance measurements. To improve the robustness and transferability of lidar intensity calibration approaches, a clearer understanding of how the laser pulse interacts with snow surface properties is needed. Here, we address this gap using a time series of UAV lidar flights conducted in the Wasatch Mountains near Sundance, Utah using a DJI M300 equipped with a Zenmuse L1 sensor. Each flight is accompanied by detailed snow pit observations and comprehensive in situ measurements of snow physical and optical properties. We apply machine learning techniques to model UAV lidar intensity returns and to quantify the relative influence of measured snow properties on the laser signal. These results provide new insight into the dominant controls on UAV lidar intensity over snow and identify key snow surface properties governing the laser-snow interaction. Together, these findings suggest a pathway toward simplified and more transferable calibration strategies that do not require coincident imaging spectroscopy. As a result, UAV lidar intensity can directly complement existing methods by enabling fine-scale snow grain size estimation independent of solar illumination.

How to cite: Ackroyd, C. and Olson, M.: Identifying Snow Surface Controls on UAV Lidar Intensity for Grain Size Retrieval, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8407, https://doi.org/10.5194/egusphere-egu26-8407, 2026.

EGU26-9074 | ECS | Orals | CR6.5

Robust Satellite Techniques for detecting and monitoring icebergs 

Iacopo Mancusi, Roberto Colonna, Carolina Filizzola, Nicola Genzano, and Valerio Tramutoli

One of the main consequences of climate change is undoubtedly rising temperatures, which cause the polar ice caps in the Arctic and Antarctic regions to melt and, as a result, icebergs to break off. Due to their high variability in shape and size, their movements and trajectories are not easy to predict, posing a threat to maritime safety and offshore activities. Particularly, along the western coast of Greenland (e. g. in the Davis Strait), in addition to the growing number of icebergs, there has also been an increase in maritime traffic, which has tripled due to the opening of new trade and tourist routes.

Historically, icebergs were detected exclusively by naval sightings or aerial patrols, which were inherently limited in terms of accuracy and unable to reach remote or inaccessible regions. In this contemporary era, advancements in satellite technology have significantly transformed the way in which icebergs are observed, ensuring high temporal and spatial resolution, global and large-scale acquisition, as well as accessible free near-real-time data. The majority of past and present studies focusing on the detection and tracking of icebergs using satellite imagery have employed fixed threshold methodologies. These tend to be prone to false alarms, offer limited sensitivity, and are not easily exportable or automatable due to their heavy dependence on observation time and location. The integration of multispectral information with diagnostic elements from a spectral perspective is a fundamental aspect of the aforementioned techniques.

In order to overcome the limitations described above, this study proposes a multi-temporal differential approach for detecting and mapping icebergs along with other objects that could potentially compromise navigation. This methodology is referred to as Robust Satellite Techniques (RST), and it has been developed to identify statistically significant variations in the signal under investigation, at the pixel level. The RST model, already widely utilised in the domain of natural hazards, is being employed for the first time in the detection of icebergs. The test was specifically conducted within a segment of the ocean in the surrounding area of Nuuk (Greenland), located in the Davis Strait. A preliminary application of the RST approach, just to the visible band of Sentinel-2/MSI, demonstrated, compared with other multi-spectral, fixed threshold approaches, higher sensitivity and reliability, together with an easy and immediate exportability in different geographic areas and observation periods. The methodology was implemented in the Google Earth Engine (GEE) environment, which allows the process to be fully automated, easily exportable and rapidly executable.

How to cite: Mancusi, I., Colonna, R., Filizzola, C., Genzano, N., and Tramutoli, V.: Robust Satellite Techniques for detecting and monitoring icebergs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9074, https://doi.org/10.5194/egusphere-egu26-9074, 2026.

EGU26-9695 | ECS | Posters on site | CR6.5

Foundation vision models for Antarctic sea ice floe segmentation and quantification from shipborne imagery 

Giulio Passerotti, Filippo Nelli, Ippolita Tersigni, Alberto Alberello, Marcello Vichi, Luke Bennetts, James Bailey, Petra Heil, and Alessandro Toffoli

Sea ice floe size, ice concentration, snow cover, and thickness collectively drive the evolution of the marginal ice zone (MIZ) by influencing albedo, melt dynamics, wave-ice interactions, ice strength, and navigation conditions for icebreakers. Yet, reliable measurements of these parameters remain scarce, significantly limiting process understanding and model validation in the Antarctic. Satellite-based products are constrained by spatial resolution, and the scarcity of ground truth data prevents thorough validation and refinement of remote sensing retrieval algorithms. We demonstrate the use of the Segment Anything Model (SAM), a foundation vision model, to extract multiple physically meaningful sea ice properties from close-range, shipborne imagery. Using extensive datasets of high-resolution images collected during multiple Antarctic icebreaker voyages, SAM identifies and delineates individual ice floes, facilitating accurate estimation of floe sizes and sea ice concentration. Validation against manually segmented benchmarks shows robust agreement across diverse ice conditions. For snow cover and ice thickness estimations, SAM is specifically fine-tuned on manually annotated datasets to detect overturning ice events, enabling thickness measurement from exposed vertical profiles, and to classify snow-covered versus bare ice, quantifying snow cover fraction on individual floes. Overall, SAM enables systematic, scalable observations previously challenging to obtain, bridging the critical sea ice data gap by transforming images into quantitative datasets that support Antarctic sea ice process studies and improve observational detail beyond satellite capabilities.

How to cite: Passerotti, G., Nelli, F., Tersigni, I., Alberello, A., Vichi, M., Bennetts, L., Bailey, J., Heil, P., and Toffoli, A.: Foundation vision models for Antarctic sea ice floe segmentation and quantification from shipborne imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9695, https://doi.org/10.5194/egusphere-egu26-9695, 2026.

EGU26-9735 | Posters on site | CR6.5

An RTK GNSS system for measuring glacier motion 

Kirk Martinez and Jane Hart

We show the development of an internet-connected GNSS to study the short-term changes in surface velocity of two adjacent Icelandic glaciers, using an RTK methodology. The system is low power, cost effective, with centimetre-level accuracy (using Ublox ZED-F9P) and transmits data to the web server daily from multiple trackers. We show that we were able to deploy trackers using a UAV (Matrice 300), which allowed inaccessible areas of the glacier to be studied. Our data indicate clear similarities in temporal velocity variations between the trackers at the individual sites, both at Breiðamerkurjökull where the units were only ~200m apart as well as Fjallsjökull where they were ~1 km apart. This demonstrates how velocity patterns were similar across the glacier.

How to cite: Martinez, K. and Hart, J.: An RTK GNSS system for measuring glacier motion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9735, https://doi.org/10.5194/egusphere-egu26-9735, 2026.

EGU26-10129 | ECS | Posters on site | CR6.5

High-Resolution Glacier Inventory Update for the Bhagirathi Basin (NW Himalaya) Using Integrated Optical and SAR Coherence Analysis 

Apoorva Malviya, Vaibhav Garg, and Rajib K. Panigrahi

Accurate monitoring of glacier extent at high spatial resolution is essential for understanding cryospheric responses to climate change, particularly in sensitive and data-sparse regions such as the Indian Himalaya. In this study, we present an updated glacier inventory for the Bhagirathi basin in the NW Himalaya using an open-source, reproducible workflow that integrates optical and Synthetic Aperture Radar (SAR) observations. The Randolph Glacier Inventory (RGI v7, ~2000) was used as the baseline dataset. Although RGI has enabled global-scale glacier assessments, its application in the Bhagirathi basin reveals spatial inaccuracies, particularly along ice divides and within debris-covered glacier zones, largely due to resolution limitations. These shortcomings were systematically addressed using high-resolution LISS-IV imagery (5.8 m) from Resourcesat-2/2A, allowing precise manual refinement of clean-ice margins and narrow glacier tongues. To improve delineation of debris-covered glaciers, we incorporated Sentinel-1A/B Single Look Complex (SLC) data from ascending and descending passes to generate interferometric coherence maps using open-source InSAR processing routines. SAR coherence, sensitive to surface motion and temporal change, proved effective in identifying actively flowing glacier ice beneath debris and in shaded terrain. Integration of coherence information with optical data significantly reduced misclassification associated with seasonal snow, surface debris, and shadow effects. The RGI baseline contained 124 glacier polygons within the Bhagirathi basin. Following detailed boundary correction and flow-divide refinement, the updated inventory identifies 103 distinct glaciers, reflecting the merging of previously mis-segmented units. The revised total glacierized area is 397.62 km², exceeding the RGI estimate due to improved detection of debris-covered ice. The updated inventory provides a robust baseline for multi-temporal glacier change analysis and demonstrates the potential of SAR-supported, high-resolution approaches for next-generation glacier inventories in the Himalaya and beyond.

How to cite: Malviya, A., Garg, V., and Panigrahi, R. K.: High-Resolution Glacier Inventory Update for the Bhagirathi Basin (NW Himalaya) Using Integrated Optical and SAR Coherence Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10129, https://doi.org/10.5194/egusphere-egu26-10129, 2026.

The Greenland Ice Sheet is a major contributor to global sea-level rise, with its mass loss raising global sea-levels by 13.59 ± 1.27 mm from 1992 to 2020. Changes to the ice dynamics of the Greenland Ice Sheet make up a significant part of this mass loss, meaning that monitoring and understanding changes in ice dynamics is crucial to assessing contemporary sea-level rise and making projections of its future.

Since 2014, the European Space Agency’s Sentinel-1 synthetic aperture radar constellation has provided near-continuous, weather-independent coverage of the Greenland Ice Sheet, with 6–12 day repeat intervals over almost all outlet glaciers. We process the full Sentinel-1 archive using an intensity feature offset tracking workflow implemented in GAMMA Remote Sensing to produce a dense, decade-spanning time series of ice velocity at 100 m resolution. This Sentinel-1 derived ice velocity dataset is extremely valuable, capturing long-term speed trends and short-term interannual variability due to seasonal drivers. However, analysing this 60 TB dataset efficiently and obtaining maximum scientific value from it is a substantial data engineering challenge, as the data volume greatly exceeds available memory quotas on HPC systems, even for relatively small geographic areas.

Here, we address this challenge with an analysis pipeline built on the Xarray, Dask, and Zarr python packages, and deployed on a HPC service. This pipeline allows both large scale interactive analysis in Jupyter notebooks, streaming to GIS software, and traditional batch processing. We leverage these tools we calculate ice-sheet wide speed change, seasonal speed variability and ice discharge in a fast, reproducible and scalable manner.

Our results reveal a highly heterogeneous dynamic response across Greenland, with neighbouring glaciers often exhibiting contrasting behaviour over the past decade. We find that short-term and seasonal variability dominates the velocity signal for most glaciers, often exceeding long-term speed changes. These findings highlight the importance of resolving short-term ice-dynamic processes when assessing Greenland’s contribution to future sea-level rise and the benefit of efficient big-data processing workflows.

How to cite: Wallis, B., Hogg, A., Rigby, R., and Slater, R.: Patterns and trends of ice dynamic variability on the Greenland Ice Sheet from a decade of high-resolution synthetic aperture radar data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11163, https://doi.org/10.5194/egusphere-egu26-11163, 2026.

EGU26-11298 | ECS | Posters on site | CR6.5 | Highlight

SAR-Driven Detection of Critical Glacial Lakes for GLOF Forecasting 

Ajay Kumar, Apoorva Malviya, and Gulab Singh

Climate warming has profoundly impacted the cryosphere of the eastern Himalaya, leading to rapid glacier retreat, the formation and expansion of proglacial lakes, and the degradation of alpine permafrost. This study examines how proglacial lakes influence the dynamics of both glaciers and rock glaciers (ice-rich debris) in the Sikkim Himalaya, with special emphasis on South Lhonak Lake. We integrate multi-temporal remote sensing datasets – including DEM differencing (TanDEM-X), optical imagery (PlanetScope), and SAR interferometry (Sentinel-1 SBAS InSAR) – to quantify landscape changes from 2016 to 2025. Results show that South Lhonak Lake expanded by ~45% in area (from ~1.12 to 1.63 km²) between 2016 and late 2023 (Qu et al., 2025), before a sudden glacial lake outburst flood (GLOF) in October 2023 drained nearly half of its volume. Pre- and post-GLOF analyses reveal accelerated glacier retreat and pronounced surface lowering at the glacier terminus adjacent to the lake. Rock glaciers in contact with the lake experienced greater surface elevation loss and deformation compared to those in non-lake settings, suggesting that thermal and mechanical erosion by the lake has exacerbated permafrost degradation. Time-series deformation mapping using SBAS-InSAR captured ongoing ground motion on periglacial slopes and rock glaciers, with line-of-sight displacement rates on the order of several cm/year in active zones. Notably, slopes fringing South Lhonak Lake showed progressive subsidence and destabilization signals before the 2023 GLOF, indicative of creeping movement in ice-rich moraine and permafrost materials. These findings highlight a coupling between proglacial lake evolution and the stability of surrounding cryospheric landforms. The study demonstrates the value of synergistic remote sensing for hazard monitoring in inaccessible high-mountain environments. It provides a first regional assessment of how an expanding (and abruptly draining) lake can influence glacier mass loss, rock glacier kinematics, and permafrost stability. Our multi-sensor approach offers a template for early detection of glacial lake outburst precursors and periglacial slope failures, information that is critical for climate change adaptation and disaster risk reduction in the Himalaya.

How to cite: Kumar, A., Malviya, A., and Singh, G.: SAR-Driven Detection of Critical Glacial Lakes for GLOF Forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11298, https://doi.org/10.5194/egusphere-egu26-11298, 2026.

EGU26-12079 | ECS | Posters on site | CR6.5

Satellite-based assessment of Getz Ice Shelf extent changes in the Amundsen Sea sector 

Aakriti Nigam and Dinesh Chandra Gupta

Antarctic Ice Shelves continuously modifies land ice and ocean boundaries and influences global climate change and sea-level fluctuations. The Getz Ice Shelf (GIS), which fringes nearly half of the West Antarctic coastline in the Amundsen Sea sector, experiences substantial basal melting. This study presents a long-term, satellite-based assessment of morphological changes in the GIS using multi-temporal austral summer (January–March) observations spanning 22-years (2003–2022). To capture spatial variability, the ice shelf was divided into three sectors (I–III) based on physiographic setting and dominant oceanographic processes, and changes in ice shelf extent were quantified along uniformly spaced transects at 5 km intervals The average of rates, end point rate, and linear regression method were employed to estimate the rate of change, with the linear regression showing the strongest correlation. Past ice shelf extents were reconstructed, and predicted ice shelf positions for the next 5 and 10 years and cross-validated with correlation coefficient and root-mean-square error. The result reveals a mean recession rate of -41.6 m/year during the austral summer of 2003–2022, and about 70% of transects show recession, while only 30% of transects are associated with progradation. LR-based projections indicate progradation in Sector I and continued recession in Sectors II and III, with pronounced retreat in Sector III between Wright Island and Martin Peninsula (~2.1 km by 2027 and ~2.5 km by 2032). Approximately 45% of transects in Sectors II and III have RMSE values of ±200 m, indicating good agreement between the estimated and satellite-based ice-shelf positions. Observed changes are linked to large-scale climate forcing, including variations in wind speed, sea surface temperature, and the Southern Annular Mode (SAM). Positive SAM and increased zonal winds may cause warm water upwelling near the Antarctic coast, impacting the extent. Changes in sea ice mass and accelerated basal melting are largely caused by ocean warming and geomorphological features, viz., bays, inlets, and islands. The study emphasizes the significant impact of ocean-atmospheric factors on Antarctic ice shelf dynamics and highlights the necessity for ongoing satellite observations and enhanced comprehension of these processes to accurately predict future changes in Antarctic ice shelves.

Keywords:

Getz Ice Shelf; West Antarctica; glacier monitoring; remote sensing; MODIS; ice shelf retreat; transect analysis; atmosphere-ocean forcings; future predictions.

How to cite: Nigam, A. and Gupta, D. C.: Satellite-based assessment of Getz Ice Shelf extent changes in the Amundsen Sea sector, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12079, https://doi.org/10.5194/egusphere-egu26-12079, 2026.

EGU26-12980 | ECS | Orals | CR6.5

A framework for evaluating ice-sheet-wide altimetry uncertainty estimates 

Karla Boxall, Malcolm McMillan, Alan Muir, Sarah Appleby, Sophie Dubber, Noel Gourmelen, Clare Willis, and Joe Phillips

Three decades of routine satellite altimetry have provided an ice-sheet-wide, near-continuous observational record of polar topography, offering unparalleled insights into ice sheet elevation change. The ability of CryoSat-2, Sentinel-3 and ICESat-2 to simultaneously and continually monitor Earth’s ice surfaces is critical towards understanding the ongoing and future imbalance of the icy continents in a changing climate. To capitalise fully on the vast quantity of altimetry data from numerous coincident missions, it is important for robust, consistent and traceable uncertainties to be provided alongside measurements of ice sheet elevation. Such information is crucial for the successful combination of measurements across missions and to enable their use in downstream applications, such as the constraint of numerical ice sheet models. At present, such uncertainties are largely absent from existing ice sheet elevation products, and for the subset of products where uncertainties are provided, there is neither a standardised approach to uncertainty generation nor a method to evaluate their robustness.

Here, we present a new framework for generating and evaluating the performance of uncertainties for altimetry-based ice sheet elevation measurements and provide a comprehensive assessment of uncertainty generation for ice-sheet-wide altimetry-based ice sheet elevation datasets. Overall, we find that calculating uncertainty as a parameterisation of topographic complexity (characterised by surface slope and roughness) and measurement quality (characterised by backscattered power and coherence) improves performance relative to solutions that use fewer co-variates. Ultimately, the framework presented here will enable the systematic characterisation of ice-sheet-wide elevation uncertainties associated with historical, current and future polar radar altimeter missions, which will be particularly important as the portfolio of polar radar altimeters continues to grow with the planned launch of the Copernicus Polar Ice and Snow Topography Altimeter (CRISTAL) in 2027. Such uncertainty information will aid the successful amalgamation of the vast array of multi-mission altimetry measurements using techniques such as Kalman Filtering and improve the constraint of numerical ice sheet models, which will in turn enable more refined estimations of current and future ice sheet mass balance and global sea-level rise.

How to cite: Boxall, K., McMillan, M., Muir, A., Appleby, S., Dubber, S., Gourmelen, N., Willis, C., and Phillips, J.: A framework for evaluating ice-sheet-wide altimetry uncertainty estimates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12980, https://doi.org/10.5194/egusphere-egu26-12980, 2026.

The rapid retreat of glaciers in the last decades highly impacts the regional hydrological cycle and water supply and increases the potential for cryosphere-related hazards. Expansion of debris-cover and changes in glacier dynamics are indicators of mass loss. While debris-cover has an insulating effect, ice-cliffs exhibit fast backwasting and therefore represent melt hotspots in the debris-covered areas. Their relative contribution has only been quantified for few glaciers and for global and regional glacier models they have therefore not yet been parameterized. The number and distribution of moulins impacts the (seasonal) glacier dynamics. Monitoring alpine glaciers is essential to quantify ongoing mass loss and project their future evolution and water supply. However, the small-scale characteristics and dynamic nature of these features cannot be captured by traditional approaches such as satellite remote sensing. Mass loss can be quantified reliably with ablation stakes at selected locations, but to investigate spatio-temporal variations across the glacier, a distributed approach is needed.

With repeated UAV photogrammetry, the  annual variability of elevation change, velocity and mass balance can be studied. On the debris-covered area, thermal imaging is employed for spatial surface temperature and debris thickness mapping. In this study, we use a structure-from-motion and multi-view stereo approach to create high-resolution orthophotos and DEMs from visual imagery of the partially debris-covered tongue of Kanderfirn in the Swiss Alps. UAV surveys have been conducted on a seasonal to annual basis since 2017 and cover the glacier tongue, which features debris-free and debris-covered surfaces. After coregistration of image pairs, we derive annual surface velocity and elevation change maps. Based on additional ice thickness information, the mass continuity method and an inversion technique is applied to investigate the glacier's dynamical evolution. The result is a SMB time-series that portrays surface processes with and without debris-cover. Additionally, the surface roughness and brightness are examined. The debris thickness maps provide a basis for estimating subdebris melt rates. Our UAV-based monitoring approach provides detailed insights into characteristic mass balance patterns and dynamic processes of (partially) debris-covered glaciers that impact their evolution and response to climatic changes. It will help with parameterizing glacier models for future mass loss projections on alpine and debris-covered glaciers.

How to cite: Zöller, A., Fürst, J. J., and Groos, A. R.: Monitoring the surface mass balance and dynamic evolution of a partially debris-covered glacier using multi-temporal visual and thermal UAV imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13044, https://doi.org/10.5194/egusphere-egu26-13044, 2026.

EGU26-13682 | ECS | Orals | CR6.5

The ESA CCI SM Freeze/Thaw Product: Global detection of frozen grounds from 1987 to the present  

Maud Formanek, Wolfgang Preimesberger, Johanna Lems, and Wouter Dorigo

The ESA CCI Soil Moisture product provides a global long-term consistent data record of soil moisture from 1978 up to the present day. It is produced by fusing measurements from a total of 19 both passive and active satellite microwave observations. Determining the physical state of water in the soil is crucial for this product, as retrievals of soil moisture are unreliable in frozen or snow-covered conditions. Beyond its role as a quality control variable, the freeze/thaw state is itself a key environmental indicator, as it impacts the exchange of energy and water between land and atmosphere, shapes seasonal hydrological cycles, and influences agriculture, ecosystems, and climate feedbacks.  

As such, as of version 9.2, the ESA CCI Soil Moisture project is providing an additional global Freeze/Thaw dataset, covering the period from November 1978 to December 2024 with daily temporal and ~25km spatial resolution. This dataset consists of a binary classification (frozen or thawed), the total number of available sensors, the number of sensors detecting frozen soils, and an agreement index for each datapoint. The product combines frozen flags from both active and passive sensors in a conservative manner, i.e. a datapoint is classified as frozen if the frozen soil classification of at least one sensor yields a positive result.  

For passive sensors, the classification of frozen soils follows a decision-tree based algorithm, which incorporates vertically polarized brightness temperature measurements at three different frequencies (Ka/K/Ku-band). These frequency bands are consistently available from 1978 onwards for all sensors included in the CCI SM product except for the L-band sensors SMOS and SMAP, which are thus excluded from the processing of the Freeze/Thaw product.  For active sensors, the surface state flag indicator provided by EUMETSAT H SAF is incorporated directly and a datapoint is marked as ‘frozen’ if its value is other than 1, which includes temporarily frozen soils, permanent ice, and melting water on the surface.   

The current product achieves an estimated accuracy of 75% against in situ surface temperature observations from ISMN and 92% compared to ERA5 reanalysis temperature fields data. The unanimity rule leads to some over-flagging and will thus be refined in future versions. Furthermore, the classification algorithm will be optimised for each sensor and its uncertainty quantified in order to merge individual classifications more robustly.   

How to cite: Formanek, M., Preimesberger, W., Lems, J., and Dorigo, W.: The ESA CCI SM Freeze/Thaw Product: Global detection of frozen grounds from 1987 to the present , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13682, https://doi.org/10.5194/egusphere-egu26-13682, 2026.

EGU26-14100 | ECS | Posters on site | CR6.5

Advances in interface detection for high-resolution snowpack analysis with (UAV-mounted) UWB radar 

Torbjörn Kagel, Aart Stuurman, Anna Siebenbrunner, Robert Ricker, and Rolf-Ole Jenssen

Snow strongly influences the climate system through its albedo and insulating properties, while also representing a critical freshwater resource. Yet, its spatial and temporal variability remain poorly constrained due to limitations of in-situ and satellite observations. Unoccupied Aerial Vehicle (UAV)-mounted surface-penetrating radars provide a solution for high-resolution snow surveys, but their data are often difficult to interpret because of variable flight conditions which, combined with the complicated EM interactions with snow, result in complex noise and signal patterns.

We present Pathfinder, an open-source algorithm for automatic detection of snow interfaces in radar echograms. The method formulates interface tracking as a path-finding problem, combining cost maps derived from reflection strength, ridge detection, and horizontal continuity, and solves it using an efficient dynamic-programming scheme. Pathfinder retrieves the air–snow and snow–ground (or snow–ice) interfaces, and can additionally identify internal layers when present. Validation against coincident in-situ snow depth measurements shows performance scores of R2 = 0.96 and RMSE = 8 cm. The algorithm is computationally efficient, enabling real-time application during surveys. Pathfinder was developed for the Ultra Wide-band Snow Sensor (UWiBaSS) from NORCE Research but we show it to be transferable across different UAV-mounted and ground-based radar systems. Case studies from Svalbard, the Alps, and Arctic- and Antarctic sea ice illustrate its robustness across diverse snow conditions. By providing a reliable, efficient, and operational interface detection method, Pathfinder advances (UAV-mounted) radar as a practical tool for snow depth and stratigraphy mapping, supporting both scientific research and in-the-field decision-making.

How to cite: Kagel, T., Stuurman, A., Siebenbrunner, A., Ricker, R., and Jenssen, R.-O.: Advances in interface detection for high-resolution snowpack analysis with (UAV-mounted) UWB radar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14100, https://doi.org/10.5194/egusphere-egu26-14100, 2026.

The mass balance estimates of the GRACE and GRACE-FO satellite missions have revolutionized our understanding of the cryosphere, yet the low spatial (~200 km) and temporal resolution (monthly) limit the detection of short-term events such as melt pulses and snowfall surges, or the onset and end of the ablation season. Furthermore, the relatively high noise at shorter time scales makes estimation of yearly mass balances challenging for the smaller glacier systems outside of the Greenland and Antarctic Ice Sheets. The MAss Change and Geosciences International Constellation (MAGIC) mission, consisting of the GRACE-C (NASA and DLR; scheduled for launch in 2028) and ESA’s Next-Generation Gravity Mission (NGGM; 2032) will drastically increase the temporal and spatial resolution of the gravimetric mass balance estimates.

Here, we combine daily surface mass balance (SMB) output from regional climate models with noise from end-to-end gravity simulations to assess NGGM and MAGIC’s capability to resolve sub-monthly mass changes over the Greenland and Antarctic ice sheets at basin scales, as well as seasonal mass balance and long-term trends of smaller glacier systems. We find that 5-daily MAGIC measurements enable the observation of extreme melt events comparable to the 2012 Greenland melt episode and capture storm-driven accumulation in Antarctica at sub-monthly time scales. For other glacier systems - such as Iceland, Patagonia, and High Mountain Asia - the mission allows the onset and termination of the ablation season to be identified within 2–3 days and constrains winter gain loss and summer mass loss to within a few gigatons, representing an order-of-magnitude improvement over GRACE(-FO). Uncertainties in long-term trends are reduced by a similar factor, such that the precision achieved by NGGM and MAGIC within a few years is comparable to that obtained by GRACE(-FO) only after 10–15 years of observations.

Overall, NGGM and MAGIC are expected to represent a step change in gravimetric cryosphere monitoring, enabling routine observation of short-term variability and supporting improved detection, attribution, and modelling of long-term mass-balance trends.

How to cite: Wouters, B. and Sasgen, I.: Advancing Observation of Cryospheric Mass Changes from sub-monthly to decadal time scales with the NGM and MAGIC Gravity Missions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14713, https://doi.org/10.5194/egusphere-egu26-14713, 2026.

EGU26-15091 | ECS | Orals | CR6.5

Extracting Swath Elevation Information from Non-Interferometric Radar Altimetry using Probabilistic Deep Learning 

Joe Phillips, Malcolm McMillan, and Jennifer Maddalena

Satellite radar altimetry provides three decades of continuous ice sheet observations, yet non-interferometric systems face a fundamental constraint: each waveform records only the return time of reflections, not their origin within the beam footprint. As a result, current approaches - which have remained largely unchanged for 30 years - rely on simplifying assumptions and fail to extract the full information content from the recorded echoes. Interferometric processing resolves this by measuring arrival angle with two antennas, enabling swath processing with multiple across-track elevation points. However, historical missions (ERS-1/2, Envisat), current operations (Sentinel-3), and planned systems (CRISTAL Ka-band) lack this capability.

Conventional processing instead eliminates ambiguity through dimensionality reduction: retracking identifies a single range from the leading edge, while slope correction locates the point of closest approach (POCA) to attribute this to. This approach discards most of the waveform information, extracting only singular elevation estimates.

Here, we present a fundamentally alternative approach to processing radar altimetry echoes over ice sheets using probabilistic deep learning to extract the distribution of plausible surface elevations encoded within each waveform. Rather than reducing ambiguity through simplifying assumptions, we treat the full waveform as exploitable information, directly modelling the distribution of surface elevations consistent with each measurement.

Specifically, we train an ensemble of 16 ResNet-RS models on 600,000 CryoSat-2 SARIn power waveforms (2012–2022) over Antarctica using the Reference Elevation Model of Antarctica (REMA) as ground truth. The framework predicts 5th, 50th, and 95th elevation quantiles across 150 points spanning the 15 km swath, providing 150 elevation estimates where conventional methods yield one. Importantly, our new probabilistic approach allows us to directly quantify both aleatoric (surface ambiguity) and epistemic (model confidence) uncertainty.

Once trained, we validated the models against unseen ice-sheet-wide REMA data (2023), demonstrating robust prediction of swath elevation distributions. Prediction interval coverage (5th–95th) averaged ~80% (10 points below the 90% nominal target) ice-sheet-wide, with consistent performance achieved with respect to ICESat-2 over Pine Island Glacier (2019–2025) - a region entirely withheld from training. The upper 95th percentile exhibited strong stability across all conditions, reflecting its physical anchoring in leading-edge returns, while lower quantiles showed systematic under-coverage increasing with topographic complexity.

Practical utility of this new approach was demonstrated through elevation change monitoring over Pine Island Glacier, where our deep learning framework reproduced established spatial thinning patterns of 2-3 m yr-1 with temporal elevation change differences of -0.03 ± 0.11 m yr-1 relative to ICESat-2. Despite using only power waveforms, performance matched CryoSat-2's interferometric POCA and EOLIS products - detecting sub-metre annual changes from probability distributions spanning tens of metres.

This represents the first swath processing from non-interferometric altimetry using power waveforms alone. By reframing waveform ambiguity as quantifiable distributional information, rather than a processing limitation, this deep learning approach demonstrates how machine learning can fundamentally rethink conventional altimetry processing, establishing new capabilities for ice sheet monitoring across past, present, and future missions.

How to cite: Phillips, J., McMillan, M., and Maddalena, J.: Extracting Swath Elevation Information from Non-Interferometric Radar Altimetry using Probabilistic Deep Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15091, https://doi.org/10.5194/egusphere-egu26-15091, 2026.

EGU26-15122 | ECS | Posters on site | CR6.5

Season-long non-destructive monitoring of snowpack surface and internal dynamics using terrestrial LiDAR and GPR 

Katrine Trottier, Baraër Michel, and Nadeau Daniel

Snowpack evolution in cold-region environments is governed by complex interactions between surface energy exchanges and internal stratigraphic processes that vary throughout the winter season. Capturing these dynamics at high temporal resolution remains challenging with conventional point-based or destructive methods. This study presents a season-long, predominantly non-destructive monitoring approach combining fixed-station terrestrial LiDAR and high-frequency ground-penetrating radar (GPR) to observe snowpack surface and internal dynamics across multiple winter processes.

Field measurements were conducted throughout the winter at two contrasting eastern Canadian watersheds. Sainte-Marthe (45°N) is a lowland agricultural catchment (110 m a.s.l.) with shallow, ephemeral snow cover, while the Montmorency Forest (47.3°N) is a boreal watershed (670 m a.s.l.) characterized by a deep, persistent snowpack. GPR systems operating at 1500 MHz and 500 MHz were deployed at Sainte-Marthe and Montmorency, respectively, to account for contrasting snow depths. A fixed 905 nm fixed LiDAR system operated concurrently at both sites, providing hourly measurements of snow surface elevation and properties. Manual snowpit surveys, including density and A2 permittivity measurements, were performed throughout the winter to constrain electromagnetic wave velocity and support GPR inversion.

LiDAR observations capture continuous changes in snow surface state, including accumulation, compaction, melt, deformation, and surface roughness, revealing periods of enhanced energy input at the snow–atmosphere interface. Corresponding variations in GPR signal amplitude, two-way travel time (TWT), and frequency content indicate internal stratigraphic adjustments within the upper snowpack layers.

Overall, integrating LiDAR and GPR with traditional monitoring stations demonstrates strong complementarity for continuous, non-destructive monitoring of snowpack processes over an entire winter season, providing new observational constraints relevant to cold-region hydrological and cryospheric modelling

How to cite: Trottier, K., Michel, B., and Daniel, N.: Season-long non-destructive monitoring of snowpack surface and internal dynamics using terrestrial LiDAR and GPR, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15122, https://doi.org/10.5194/egusphere-egu26-15122, 2026.

EGU26-16192 | Orals | CR6.5

Scalable satellite data processing methods for ICESat-2, optical stereo and SAR/InSAR to understand cryosphere change 

David Shean, Joseph-Paul Swinski, Eric Gagliano, George Brencher, Hannah Besso, and Scott Henderson

Modern constellations of Earth observation satellites offer exciting opportunities to observe and understand cryosphere change with unprecedented spatial and temporal coverage, resolution, and accuracy. This ever-growing data firehose requires new scalable processing approaches to extract local, regional, and global results and actionable insights for downstream applications. Mulit-modal data fusion (e.g., integration of commercial very-high-resolution optical stereo, laser altimetry, and high-resolution SAR/InSAR) can capture mm- to meter-scale surface change, offering new insight for a range of geophysical processes responsible for cryosphere change.

We highlight a set of scalable, open-source satellite data processing tools and approaches for high-mountain cryosphere science applications, including:

1) Sliderule Earth - an open-source service for on-demand, parallel processing of science data archives in the cloud. SlideRule allows the user to create customized, high-level, analysis-ready data products in near-real-time. SlideRule currently supports a suite of data products and algorithms for the NASA ICESat-2 and GEDI satellite laser altimetry missions, as well as many cloud-hosted raster datasets (e.g., PGC ArcticDEM/REMA strips and mosaics, Harmonized Landsat-Sentinel, ESA WorldCover 10m, USGS 3DEP airborne lidar).

2) Intra- and interannual snow depth measurements from ICESat-2 satellite laser altimetry and commercial optical stereo

3) Global annual high-resolution snow melt runoff onset maps for the past decade from the cloud-hosted archive of radiometric terrain-corrected (RTC) Sentinel-1 SAR backscatter

4) Fused InSAR and SAR feature tracking to map debris-covered ice and evolving high-mountain hazards, including the seasonal and interannual motion of glacier lake moraine dams.

These satellite datasets and approaches offer an improved understanding of the processes driving recent cryosphere change, which is essential to improve the models used for future projections, and to understand connections with the hydrologic cycle.

How to cite: Shean, D., Swinski, J.-P., Gagliano, E., Brencher, G., Besso, H., and Henderson, S.: Scalable satellite data processing methods for ICESat-2, optical stereo and SAR/InSAR to understand cryosphere change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16192, https://doi.org/10.5194/egusphere-egu26-16192, 2026.

EGU26-16858 | Orals | CR6.5

From field photos to microscope images: a low-cost toolbox for glacier surface darkening and biological impurity analysis 

Alexandre Anesio, Shunan Feng, Beatriz Gill Olivas, Emily Louise Mary Broadwell, Ravi Sven Peters, Liane G. Benning, and Martyn Tranter

The albedo lowering of glacier and ice sheet surface is driven by a complex combination of biogeophysical processes, including the accumulation of biologically active impurities such as glacier ice algae and dispersed cryoconite. It is therefore important to understand darkening processes by ground observations and sampling. In situ sampling requires a simple yet effective approach to quantify surface ice darkness and estimate the possible range of impurity concentrations. Traditional post-processing of snow and ice samples for cell and mineral counts can also be time and resource consuming.

In this study, we present a novel toolbox for calibrating field images acquired with consumer-grade cameras (e.g., smartphones or digital cameras) to estimate surface ice darkness. Using a data-driven approach, we tested the method on snow and ice samples collected in Greenland to predict impurity ranges. The toolbox also integrates advanced AI models for automated segmentation of microscope images and classification of snow algae, glacier ice algae, and mineral particles, enabling rapid impurity quantification. The new toolbox can enable researchers across fields to cross compare fieldwork samples. It also offers potential for integration into automated weather stations for long-term monitoring programs, advancing glacier surface darkening characterization and biogeophysical research.

How to cite: Anesio, A., Feng, S., Olivas, B. G., Broadwell, E. L. M., Peters, R. S., Benning, L. G., and Tranter, M.: From field photos to microscope images: a low-cost toolbox for glacier surface darkening and biological impurity analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16858, https://doi.org/10.5194/egusphere-egu26-16858, 2026.

Glaciers in the Alps are receding at unprecedented rates. Firn area is declining even at high elevations and many glaciers have experienced completely snow free summers in recent years. Glacier albedo is an important control for the amount of energy available for melt and, hence, mass balance and future glacier evolution. Glacier-scale studies have shown considerable variability of glacier-wide and bare-ice albedo in both space and time. At regional and Alps-wide scales, analyses of MODIS data have found decreasing albedo trends over time. However, the relatively coarse resolution of MODIS (500 m) does not resolve small-scale variability and limits applicability especially for very small glaciers, which are numerous in the Alps. Deriving glacier-wide albedo products and addressing albedo variability over bare-ice areas using Landsat and Sentinel-2 multispectral surface reflectance (10 to 30 m resolution) has the potential to improve understanding of albedo driving factors and, for example, resolve regional impacts of heatwaves and other meteorological forcings. Landsat and Sentinel-2 surface reflectance products are available via Google Earth Engine (GEE) and the computational accessibility enabled by server-side operations within GEE allows flexible analyses at scale. For example, a glacier-wise analysis of the Sentinel-2 record indicates that the median snow cover fraction for glaciers in Austria dropped to around 10 % during the record-breaking summer of 2022, compared to values between 20 and over 30 % in the previous years. Applying a broadband albedo conversion to the multispectral reflectance data, we find the median glacier area fraction with very low albedo values below 0.2 increased to over 35 % in 2022. At elevations above 3000 m, median glacier albedo ranged from 0.4 to 0.5 in years prior to 2022 and dropped to below 0.3 in 2022, with persistently low values through 2025.

In principle, these GEE workflows can be scaled to much larger regions and thousands of individual glaciers without great difficulties. However, “traditional” challenges related to cloud cover, local topographic shading, data availability, and validation approaches remain. It has become relatively simple to produce values like the preliminary results given above and, for example, greatly extend the dataset by including the entire Landsat record. However, given the large amount of readily available data across different collections and generations of satellites, care should be taken in accounting for issues such as sensor comparability and level-2 product consistency, and developing meaningful validation metrics seems particularly important. We will present our ongoing work related to ice albedo and firn loss in the European Alps and aim to foster discussions of challenges and limitations that arise when scaling analyses from individual glaciers to larger regions. 

How to cite: Hartl, L., Di Mauro, B., Fugazza, D., and Naegeli, K.: Deriving glacier albedo time series from multispectral satellite data in the Alps - insights and challenges from regional applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17314, https://doi.org/10.5194/egusphere-egu26-17314, 2026.

EGU26-17377 | ECS | Orals | CR6.5

Optimizing SAR for Glacier Mapping: A Resolution-Weighted Coherence and Backscatter Dataset of the European Alps 

Luis Q. Gentner, David Small, Livia Piermattei, and Hendrik Wulf

Accurate and up-to-date glacier outlines are essential for quantifying glacier retreat and enabling downstream applications, such as mass balance assessments and glacier modeling. While manual delineation of glaciers remains common, automated approaches offer faster and more consistent mapping. However, even sophisticated deep learning methods show limited performance on debris-covered glaciers, which are difficult to differentiate from periglacial terrain. Optimizing input features is a key strategy to overcome this barrier. Synthetic Aperture Radar (SAR) interferometric coherence complements optical data effectively, as moving ice surfaces typically exhibit lower coherence than stable terrain.

We present a new dataset covering glaciated areas of the European Alps from 2015 to 2025, consisting of annual composites of Sentinel-1 coherence and backscatter. We have developed an automated pipeline to process multiple TB of Sentinel-1 Single Look Complex (SLC) data. For each year, bursts acquired during minimal snow cover were selected and combined to ensure optimal visibility of glacier ice. Backscatter was radiometrically terrain-flattened, and both coherence and backscatter were geocoded to the UTM coordinate system. To mitigate the high spatial resolution variability inherent to SAR imaging in mountainous terrain, we applied the local resolution-weighting approach (Small, 2012). This method combines ascending and descending acquisitions, weighting contributions by the inverse of the local contributing area to preserve the highest resolution available.

The resulting dataset provides analysis-ready annual composites at 10 m grid spacing and will be made publicly available. This enables the development and benchmarking of more robust glacier mapping methods across the European Alps, particularly in challenging debris-covered areas.

How to cite: Gentner, L. Q., Small, D., Piermattei, L., and Wulf, H.: Optimizing SAR for Glacier Mapping: A Resolution-Weighted Coherence and Backscatter Dataset of the European Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17377, https://doi.org/10.5194/egusphere-egu26-17377, 2026.

EGU26-18761 | ECS | Posters on site | CR6.5

A Deep Active Learning Framework for the Detection of Subsurface Meltwater Lakes on Antarctic Ice Shelves 

Paula Suchantke, Rebecca Dell, and Neil Arnold

The Antarctic Ice Sheet is the largest potential contributor to future global sea level, with a maximum contribution of approximately 58 m. The flow of grounded ice towards the ocean is largely restricted by floating ice shelves, which fringe ~75% of the Antarctic coastline. This buttressing effect can be diminished or lost entirely following partial or complete ice-shelf disintegration events, leading to an acceleration of ice discharge. The vulnerability of ice shelves to fracture and disintegration is influenced by a range of factors, including the ponding of surface and subsurface meltwater, which can induce flexural stresses and promote fracture through the ice-shelf column.

While the widespread extent of surface meltwater systems across numerous Antarctic ice shelves during the austral summer is now well documented, meltwater storage within the ice-shelf subsurface remains poorly understood. Liquid water can persist perennially beneath the ice-shelf surface if sufficiently insulated by surrounding and overlying layers of firn, snow, and/or ice. Due to their year-round persistence, buried meltwater lakes introduce a potential mechanism for hydrofracture outside of the melt season, with important implications for ice-shelf stability.

In situ surveys in Antarctica are logistically challenging and limited in spatial extent, rendering spaceborne remote sensing an indispensable tool for monitoring ice-shelf processes at a continental scale. However, the growing volume of satellite observation poses data-analysis challenges typical of the ‘Big Data’ era; remote-sensing datasets are often high-dimensional, unstructured, and large in sample size, with rapidly increasing spatiotemporal coverage and low-cost availability. These characteristics limit the scalability of manual interpretation or traditional thresholding approaches for pan-Antarctic applications. In contrast, machine-learning methods are ideal for extracting patterns and features from large databases of satellite imagery. In light of this, machine learning offers great potential for the detection of subsurface meltwater across Antarctic ice shelves at a continental scale, if challenges relating to the sampling and labelling of training data, as well as class imbalance, are addressed carefully. An active learning strategy can help to reduce data redundancy and labelling requirements in deep learning, while also improving model performance in the presence of class imbalance.  

Here, we present a systematic training-data sampling strategy applied to all major Antarctic ice shelves. We employ a stratified random sampling approach to mitigate strong regional imbalances in data availability and create a curated training data subset that combines an equal number of random and expert-selected samples. This dataset is used to initialise an active learning framework for training a deep-learning model to detect subsurface lakes in Antarctica. We evaluate model performance across multiple configurations and present fine-tuning of model hyperparameters.  

How to cite: Suchantke, P., Dell, R., and Arnold, N.: A Deep Active Learning Framework for the Detection of Subsurface Meltwater Lakes on Antarctic Ice Shelves, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18761, https://doi.org/10.5194/egusphere-egu26-18761, 2026.

EGU26-20200 | Posters on site | CR6.5

InSAR Svalbard Ground Motion Service  

Emma Hauglin, Gökhan Aslan, Marie Bredal, Line Rouyet, John Dehls, Tom Rune Lauknes, Lotte Wendt, Daniel Stødle, Heidi Hindberg, Jetle von Oostveen, and Yngvar Larsen

InSAR is a key technology for monitoring ground movements such as subsidence, uplift, unstable slopes, and natural hazards, and it plays a critical role in reducing risks to infrastructure and communities. Since the launch of InSAR Norway in 2018 and European Ground Motion Service (EGMS) in 2022, these datasets have been freely available. However, Svalbard has not been covered by any of these services. With temperatures rising at a rate seven times faster than the global average, the need for consistent and long-term InSAR data in Svalbard and the Arctic is evident.

With funding from the Norwegian Space Agency and in collaboration with NORCE, the Geological Survey of Norway (NGU) launched the InSAR Svalbard Ground Motion Service in February 2026. The pilot products provide the first open-access InSAR dataset for Svalbard using Sentinel-1 data. Tailored to Arctic conditions, the service offers (1) seasonal data during snow-free periods aimed to detect fast-moving areas and to monitor seasonal patterns, and (2) interannual data between snow-free periods to monitor slower ground motion. It delivers essential data for monitoring permafrost degradation, slope creep processes, and freeze-thaw processes, providing critical information for research and risk management.

The pilot products are currently available for selected areas around settlements and research stations and are accessible through a web-GIS platform that provides easy visualization and analysis tools. Future development will expand coverage across the entire archipelago, integrate new satellite data, and progress towards a comprehensive ground and ice motion service.

How to cite: Hauglin, E., Aslan, G., Bredal, M., Rouyet, L., Dehls, J., Lauknes, T. R., Wendt, L., Stødle, D., Hindberg, H., von Oostveen, J., and Larsen, Y.: InSAR Svalbard Ground Motion Service , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20200, https://doi.org/10.5194/egusphere-egu26-20200, 2026.

EGU26-2483 | ECS | Orals | CR6.8

Global Patterns of Soil Freeze-Thaw States Below 0 °C 

Zhaoyu Dong and Yuanchao Fan

Accurate prediction of permafrost thaw requires understanding soil freeze-thaw dynamics, yet current climate models assume pure water freezing points that may be inadequate for real soils. Traditional freeze-thaw theory suggests that salt in soil water increases Gibbs free energy, lowering the soil freezing point and enabling sub-zero unfrozen states (SUS). While these physical and chemical interactions have been documented in laboratory studies, they have not been evaluated by large-scale Earth observations. Here, by integrating satellite-derived freeze-thaw states with soil property datasets, we investigated thermal dynamics and mechanisms of SUS events across seasonally frozen soils of the Northern Hemisphere using machine learning and statistical analyses. Using satellite observations, we estimate a representative soil freezing point of 271.83 K, characterized by the median temperature of first seasonal freezing, which is nearly 1.3 °C lower than that of pure water. SUS events showed a wide occurrence temperature range (interquartile: 269.04–272.74 K), with 37.67% occurring at temperatures below the median freezing point. These low-temperature events are mainly driven by soil salinity and spontaneous entropy-increasing thawing processes. We compared observed freezing point depression with a simple physicochemical model incorporating soil salinity and moisture effects, which demonstrated strong agreement. These findings suggest that climate models assuming a 0 °C freezing point may underestimate active layer thawing rates and permafrost degradation risks. Our results indicate an urgent need to incorporate freezing point depression in Earth system models to accurately predict permafrost stability, with important implications for climate projections and ecosystem management.

How to cite: Dong, Z. and Fan, Y.: Global Patterns of Soil Freeze-Thaw States Below 0 °C, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2483, https://doi.org/10.5194/egusphere-egu26-2483, 2026.

EGU26-2956 | Orals | CR6.8

Changes in sub-glacial and bedrock hydrology by retreating glaciers in Svalbard 

Thomas Zwinger, Andrew Hodson, and Tristram Irvine-Fynn

The ongoing retreat of glaciers in Svalbard potentially exposes a permafrost-free glacier forefield (talik), which in certain cases also can become exploited by CH4-saturated groundwater.  In order to understand potential gas transfer to forefields linked to changing groundwater recharge and subglacial pressures, we present a coupled model for ice-dynamics, sub-glacial water flow and a geo-thermal groundwater-permafrost model, all included and coupled together in the package Elmer/Ice. The thermo-mechanical ice-flow problem is solved using the Stokes equations, sub-glacial hydrology by GlaDS.  With the additional geo-thermal groundwater-permafrost model we are in a position to study the complete transient hydrological and thermal system from glacier surface - with prescribed moulin recharge - down to the sub-permafrost aquifer and can trace groundwater paths with a seasonal resolution. Along the well studied glacier Midtre Lovénbren we demonstrate the importance of producing consistent initial conditions (in particular for permafrost distribution) and show transient simulation results that are qualitatively able to reproduce observed seasonal outflows of subglacial water in the glacier forefield.

How to cite: Zwinger, T., Hodson, A., and Irvine-Fynn, T.: Changes in sub-glacial and bedrock hydrology by retreating glaciers in Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2956, https://doi.org/10.5194/egusphere-egu26-2956, 2026.

EGU26-5285 | Orals | CR6.8

DTC Ice Sheets: Regional Sea Level Fingerprints from EO-Constrained Mass Balance 

Sebastian B. Simonsen and the DTC Ice Sheets Team

As ice sheets melt, they contribute to sea level rise, a process that varies regionally due to gravitational, rotational, and deformational effects, making location-specific projections essential for effective coastal adaptation. Here, we present the Mass Balance and Sea Level module of the ESA Digital Twin Component (DTC) for the Ice Sheets system, which is developed as a precursor to ice efforts within the EU's Destination Earth (DestinE) platform.

Our approach integrates multi-decadal radar altimetry observations and land surface temperature records to diagnose the contemporary ice sheet mass balance for Greenland, based on machine learning techniques to capture fine-scale spatial patterns in mass change. Additionally, our sea-level module computes regionally resolved sea level fingerprints that account for far-field effects of ice sheet mass redistribution, translating ice sheet changes into location-specific projections along European coasts.

Here, we demonstrate the operational capability through scenario-based applications, quantifying how different mass loss pathways affect coastal regions distinctly across Europe. Further, the system's modular architecture also enables interoperability with ocean and atmosphere components within DestinE, when ready, supporting integrated what-if scenario exploration.

Ultimately, by operationalizing the connection between satellite observations and regional sea level projections, the DTC Ice Sheets module may help bridge the observational-modeling divide and provide stakeholders with actionable insights for climate adaptation.

How to cite: Simonsen, S. B. and the DTC Ice Sheets Team: DTC Ice Sheets: Regional Sea Level Fingerprints from EO-Constrained Mass Balance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5285, https://doi.org/10.5194/egusphere-egu26-5285, 2026.

Deglaciation, declining seasonal snow cover, and permafrost thaw are among the most visible consequences of climate change. Yet, the implications of these cryosphere changes for river runoff—and for practical water management—remain insufficiently quantified. This study contributes to a broader initiative aimed at comprehensive assessment of past and future climate-driven changes in snow- and ice-dominated regions.

We applied graphical–analytical hydrograph separation into genetic runoff components (baseflow, spring snowmelt, rainfall floods, thaw floods) to 94 gauging stations from the Norwegian Streamflow Reference Dataset for 1960–2024, using the grwat R package. Daily discharge was combined with watershed-averaged daily precipitation and air temperature from the ERA5 reanalysis as input. We identify two key hydrograph transformations associated with cryosphere change: (1) a reduction in the volume of the spring snowmelt flood (vårflom) and (2) an intensification of winter thawing processes. The latter manifests as either higher runoff volumes during episodic winter thaw and rain-on-snow floods, or an increase in the frequency and duration of thaw-flood events, particularly since the 1990s–2000s.

As many Norwegian hydropower reservoirs were designed to capture spring snowmelt and release water during winter, these shifts imply increasing mismatch between inflow seasonality and existing regulation strategies. Possible operational tensions include reduced spring refill reliability, higher winter spill risk, or changing flood-control constraints. The observed trends therefore highlight a need to adapt reservoir operations to the likely continued redistribution of runoff from spring toward winter.

The study was funded by the European Union’s Horizon Europe research and innovation programme through the project LIQUIDICE (grant number: 101184962). 

How to cite: Rets, E., Woods, R., Osuch, M., and Luks, B.: Detecting Cryosphere Signals in Runoff: Trends in Genetic Components in Norwegian Reference Streamflow and its Implication for Norwegian Hydropower Regulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9937, https://doi.org/10.5194/egusphere-egu26-9937, 2026.

EGU26-10991 | ECS | Posters on site | CR6.8

Dynamic simulations of Icelandic ice cap evolution constrained by observations 

Louise Steffensen Schmidt, Guðfinna Aðalgeirsdóttir, Joaquín M.C. Belart, and Brice Noël

Like most ice caps and glaciers worldwide, Icelandic glaciers are losing mass and retreating as a result of a warming climate. Here, we link satellite observations and dynamic ice-flow modeling to produce robust long-term projections of the five largest Icelandic ice caps—Vatnajökull, Langjökull, Hofsjökull, Mýrdalsjökull, and Eyjafjallajökull—until 2300 under the RCP 8.5 scenario. The simulations are conducted using the Parallel Ice Sheet Model (PISM), forced by climatic mass balance fields from a regional climate model.

PISM is initialized by constraining ice-flow parameters using satellite-derived surface velocities from Sentinel-1 for the period 2015–2020. Simulated velocities are compared to observations to identify the best-fitting parameter set, and simulated thickness and area changes are evaluated against available geodetic measurements and glacier outlines. These observational constraints are used to improve confidence in subsequent long-term projections.

The calibrated ice-flow model is then used to simulate glacier evolution until 2100, and then the 2081–2100 climatic mass balance forcing is repeated to extend the simulations to 2300. The ice caps are projected to lose 15–30% of their volume and 7–22% of their area by 2100, increasing to 50–70% volume loss and 30-60% area loss by 2300.

How to cite: Schmidt, L. S., Aðalgeirsdóttir, G., Belart, J. M. C., and Noël, B.: Dynamic simulations of Icelandic ice cap evolution constrained by observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10991, https://doi.org/10.5194/egusphere-egu26-10991, 2026.

EGU26-12264 | Posters on site | CR6.8

Brine flow in permafrost, time constraints by Ra isotopes  

Yishai Weinstein, Dotan Rotem, Yehudit Harlavan, and Hanne H. Christiansen

The archipelago of Svalbard, at 76-80oN, is located at the heart of the continuous permafrost zone, which means that all exposed areas (glacier-free) are covered by 100-400m thick permafrost. Permafrost in valleys is often saline due to Early Holocene seawater ingression, followed by regression and permafrost aggradation. We studied the chemistry and Ra isotopes of ground ice from saline permafrost at the Adventdalen valley, central Svalbard. Cores recovered from two adjacent drillholes, 10 km from the sea, within the Early Holocene seawater ingression, showed significantly different compositions. While one core, with up to seawater salinity, showed similar-to-seawater composition, ground ice in two less saline cores exhibited clear evidence for water-rock interaction. The cores also showed substantial differences in their radium isotopes. Ratios of long to short-lived isotopes (e.g. 226Ra/223Ra) in the ground ice of the less saline cores were much higher than in the more saline one (activity ratios of <<20 and >20, respectively). Notably, Ra isotope ratios in the latter were similar to (i.e. in secular equilibrium with) the ratios of their radioactive parents (e.g. 230Th/227Ac) on sediment surfaces (CEC fraction), while in the less saline cores, ratios were closer to parent ratios in the bulk sediments.  

Another drillhole, 5 km from the sea, intruded a cryopeg (permafrost with overcooled brines),  with hypersaline ground ice from 20m to 4m below surface and brine (50,000mg Cl l-1) that flowed into the borehole at a depth of 11m. Composition of both brine and the ground ice was indistinguishable from that of seawater, indicative of freezing-associated solute rejection with no crystallization or water-rock interaction involved. Importantly, (226Ra/223Ra) activity ratios in brine and the ground ice were significantly lower than the equilibrium ratios (mostly <<10).  

It is suggested that the high (226Ra/223Ra) ground ice of the less saline cores represent the original Early Holocene sediment fluids, which had interacted with sediments, diluted and froze upon exposure to the atmosphere. On the other hand, the low (226Ra/223Ra) ground ice of the more saline cores is evidently much younger (no time for diffusion of the long-lived 226Ra from inside the grains), probably produced by Late Holocene brine infiltration from the underlying basement, which is evident in the brine found in the second site.

These observations demonstrate the complex history of permafrost and its liability to fluid migration. This further highlights another aspect in permafrost’s vulnerability and sensitivity to the ongoing climate change and warming. 

How to cite: Weinstein, Y., Rotem, D., Harlavan, Y., and Christiansen, H. H.: Brine flow in permafrost, time constraints by Ra isotopes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12264, https://doi.org/10.5194/egusphere-egu26-12264, 2026.

EGU26-12418 | Orals | CR6.8

Energy-balance modeling of glacier mass balance in Iceland 

Tarek Zaqout, Bolli Pálmason, and Tómas Jóhannesson

The detailed, physically-based, one-dimensional snowpack model SURFEX/ISBA-Crocus was used to simulate the seasonal and annual surface mass balance (SMB) of the five largest Icelandic glaciers (Vatnajökull, Langjökull, Hofsjökull, Mýrdalsjökull and Drangajökull) for the period of 1990–2024, for which annual mass-balance measurements are available. The model is forced using the high-resolution Copernicus Arctic Regional Reanalysis (CARRA) dataset. Near-surface air temperature from CARRA was downscaled using a daily lapse rate (multi-year average for each day of the year) using Digital Elevation Models (DEM) with 100-m or 250-m resolution. In addition, a precipitation/elevation gradient of 10% per 100 m was applied using the elevation difference between the higher-resolution DEM and the CARRA DEM following a reclassification of rainfall and snowfall to take into account the downscaled temperature. Daily albedo from the Moderate Resolution Imaging Spectroradiometer (MODIS), data for 2000–2024, and observations from the Icelandic Glacier Automatic Weather Station (ICE-GAWS) network, data for 2001–2024, as well as the glacier mass-balance data, are used to calibrate the model. An intermediate complexity modeling strategy was considered in this work, which takes into account the effect of light absorbing particles (LAP) on albedo using an LAP-informed and spatially variable snow-darkening coefficient to control the time evolution of snow albedo in the visible range. Roughness length of pure snow (Z0snow) in the range of 0.1–10 mm was also used as a calibration parameter. Multi-year mean albedo values from MODIS were calculated for the period of 2000–2017 to represent the end-of-summer ice albedo, used as inputs to the model at each of the SMB measuring stakes. The modeled seasonal and annual SMB results were compared to measurements at more than 150 stakes on the five glaciers. Summer and winter mass balances were well predicted by the model (the model explains 70–80% of the variance, RMSE = 0.6–0.9 m w.e.). The modeled albedo was compared with the observed albedo values from MODIS and ICE-GAWS data. The model captures the temporal evolution of albedo relatively well, but generally underestimates high albedo values and overestimates low albedo values. The model was also not able to capture variability in ice albedo during the ablation season due to the use of a constant multi-year average ice albedo, which results in an underestimation of the highest melt values. Further improvements in the model are under development, including a correction of the multi-year late-summer ice albedo from MODIS to improve summer melt estimation.

How to cite: Zaqout, T., Pálmason, B., and Jóhannesson, T.: Energy-balance modeling of glacier mass balance in Iceland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12418, https://doi.org/10.5194/egusphere-egu26-12418, 2026.

The Polar Regions in the Earth System (PolarRES) project financed by the European Union’s Horizon 2020 research and innovation programme involved more than 80 researchers from 21 organisations across Europe, Asia, and North America. The project, which began in September 2020 produced an ensemble of high-resolution regional climate simulations for the Arctic and Antarctic in support of impact assessments in the polar regions. These simulations from the PolarRES project used a novel storylines approach and a multi-disciplinary framework to develop century-long climate projections at spatial scales of approximately 12km which is unprecedentedly high resolution for any multi-model ensemble covering the Arctic for such a long period of time. The PolarRES ensemble followed the CORDEX protocol and are publicly available for the wider scientific community. In this talk, I will present an overview of the PolarRES simulations, their performance, and show some recent applications of these climate simulations for studying the impacts of future climate change in the Arctic.

How to cite: Mooney, P.: Storylines of Arctic Climate Change: High-resolution climate projections for the Arctic , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12816, https://doi.org/10.5194/egusphere-egu26-12816, 2026.

EGU26-13370 | Posters on site | CR6.8

How well do global reanalyses estimate snow density? 

Colleen Mortimer, Lawrence Mudryk, and Vincent Vionnet

Snow density is critical to the accurate simulation of energy exchange between the atmosphere and the underlying soil. Along with snow water equivalent (SWE) it is a key constraint on snow depth (HS). The snow density formulations used in global reanalyses have been developed and validated using detailed observational datasets but often from very limited locations. Unlike SWE and HS from global climate reanalyses which have been comprehensively evaluated using in situ observations, to our knowledge there are no similar hemispheric-scale assessments of snow density from these products. To address this gap, we use snow course observations from the NorSWE dataset to simultaneously evaluate SWE, SD, and snow density in five reanalysis products (ERA5, ERA5-Land, GLDAS2.1 Noah, JRA-3Q, MERRA2). We consider snow across the Northern Hemisphere over a range of snow classes and assess its seasonal evolution across the snow onset, peak and melt periods.

Results show a large spread in snow density both in terms of its spatial pattern and average magnitude. Products that can reasonably estimate SWE and/or HS do not necessarily have accurate snow density representations and vice versa. For example, MERRA2 ranks in the middle of the assessed products in terms of SWE and HS skill but its snow densities are poorly correlated with observations, whereas GLDAS 2.1 (Noah 3.6) has some of the largest SWE and HS errors, but some of the smallest snow density errors. Inaccuracies in SWE, HS and density can compensate for each other in different ways and these relationships vary between reanalyses. By examining snow density alongside SWE and HS, we aim to diagnose the principal sources of error in reanalysis snow estimates as stemming from errors in the snow model and its structural implementation within the reanalysis or from biases in meteorological forcing.

How to cite: Mortimer, C., Mudryk, L., and Vionnet, V.: How well do global reanalyses estimate snow density?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13370, https://doi.org/10.5194/egusphere-egu26-13370, 2026.

EGU26-13566 | ECS | Posters on site | CR6.8

In situ measurements of ice growth and melt in two lakes of eastern Canada to improve ice representation in the Canadian Small Lake Model 

Thomas Brady, Antoine Thiboult, Tadros Ghobrial, Murray Mackay, and Daniel F. Nadeau

In cold regions, lake ice, which persists for months, influences the exchange of heat, momentum, and water between the earth’s surface and the atmosphere. Several lake models have been developed for simulating these exchanges, such as the Canadian Small Lake Model (CSLM) - a one-dimensional physical lake model that represents the thermal structure of lakes and their exchange of energy with the atmosphere, including the formation and evolution of ice and snow cover. These models do not always adequately simulate important parameters such as ice thickness, which in turns makes model evaluation an important, yet difficult task. The main challenge with model evaluation is the limited amount of observational data, since most northern lakes are in remote areas with limited accessibility.

This study presents an analysis of the temporal evolution of ice cover in two northern lakes over two winters and compares in situ measurements with the CSLM.

Field data were collected using an innovative temperature profiler. During the 2024-2025 winter, two profilers were deployed on two lakes in the boreal biome of Quebec, Canada: Piché Lake (0.15 km²; mean depth 2.2 m; ~47°N), a small lake surrounded by topography that facilitates snow accumulation leading to snow-ice formation, and Bernard Lake (4.6 km²; 13 m; ~51°N), a larger, more wind-exposed lake where thermal ice formation is dominant. During the 2025-2026 winter, only one profiler was deployed at Piché Lake. Profiler data were processed to generate a continuous dataset of ice and snow thickness for comparison with the CSLM outputs. The simulation was validated through manual measurements of ice and snow thickness at both Bernard and Piché Lakes, as well as upward-looking sonar measurements at Bernard Lake. Additional information on snow and ice properties was collected using snow pits, ice core sampling and visual observations using a GoPro camera, providing a more comprehensive basis for assessing and improving the representation of snow and ice processes in the CSLM.

Preliminary comparisons with CSLM indicate that the model generally underestimates maximum lake ice thickness. Also, the model predicts freeze-up earlier than observed, while it predicts breakup either earlier or later than observed. The contrasting ice processes at Piché and Bernard lakes, characterized by dominant snow-ice and thermal ice formation, respectively, provide a useful basis for evaluating the performance of the snow-ice production module in the model. Planned comparisons of snow cover will refine the module and improve the model’s representation of snow and ice.

Overall, this work advances understanding of atmosphere–cryosphere interactions and provides recommendations to improve CSLM performance.

How to cite: Brady, T., Thiboult, A., Ghobrial, T., Mackay, M., and Nadeau, D. F.: In situ measurements of ice growth and melt in two lakes of eastern Canada to improve ice representation in the Canadian Small Lake Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13566, https://doi.org/10.5194/egusphere-egu26-13566, 2026.

EGU26-15193 | Posters on site | CR6.8

Continuous Weather Observation under extreme conditions – Antarctica 

Ahmed Al Kaabi, Badr AlAmeri, Muhammed Haroon, and Petar Sapundjiev

During the 33rd Bulgarian Antarctic expedition, the National Center of Meteorology (NCM), United Arab Emirates, successfully installed 365 days around the year, first UAE advanced automatic weather station on Livingstone Island, Antarctica.  The station is equipped with ten high precision sensors, including air temperature (three thermometers), wind speed and direction, barometric pressure, relative humidity, global solar radiation, cumulative ultraviolet radiation, and satellite-based iridium communication for real-time data transmission.

The primary objective of this installation is to provide continuous, high-resolution meteorological observations under extreme Antarctic conditions, enabling detailed monitoring and analysis of local and mesoscale atmospheric processes. These observations contribute to a better understanding of climate variability and change in the Antarctic region, which plays a critical role in the global climate system.

In addition, the collected data supports regional and global scientific research initiatives by contributing to the international datasets and numerical weather predictions (NWP) models and Artificial Intelligence within the World Meteorological Organization (WMO) framework. This integration aims to enhance weather forecasting accuracy, early warning systems, and nowcasting capabilities, particularly for polar and downstream mid-latitude regions and furthermore.

The station also supports interdisciplinary research by providing valuable observations for studies related to atmospheric dynamics, surface-atmosphere interaction, glacier behavior, and potential links with seismic and volcanic activity. Through collaboration with international Antarctic research institutions and scientists, this initiative strengthens global partnerships, improves data sharing and addresses critical observational gaps in one of the world's most data-sparse environments.

This deployment represents a significant step toward long-term environmental monitoring in Antarctica and reinforces the UAE’s contribution to global climate research, early warning systems and informed decision-making for planetary protection through the Emirates Polar Program. This was UAE’s first step and more actions to climate is in progress.

How to cite: Al Kaabi, A., AlAmeri, B., Haroon, M., and Sapundjiev, P.: Continuous Weather Observation under extreme conditions – Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15193, https://doi.org/10.5194/egusphere-egu26-15193, 2026.

EGU26-18102 | ECS | Orals | CR6.8

Magnitude and controls of snow sublimation at a high-elevation Swiss alpine site  

Isabella Anglin, Ryan Teuling, Marius Floriancic, Patricia Asemann, Michael Lehning, and Harsh Beria

Snow sublimation remains poorly quantified globally, with published estimates spanning orders of magnitude (≈0.01mm/day to >6mm/day), corresponding to ~ 5-90% of winter snowfall. This large uncertainty limits our ability to accurately quantify water availability to downstream ecosystems, as vapor losses through sublimation reduce meltwater availability. Here, we quantify surface snow sublimation over one full winter season (November 2024 to June 2025) at a high-elevation alpine site (Weissfluhjoch Versuchsfeld, 2455 m a.s.l., Switzerland) using continuous eddy-covariance measurements from an integrated open-path gas analyzer and sonic anemometer (IRGASON). We applied an eXtreme Gradient Boosting (XGB) model to estimate surface snow sublimation and used TreeExplainer-based Shapley Additive Explanations (SHAP) to quantify the relative importance of different meteorological variables on modeled sublimation.

Over the 2024-25 winter season, cumulative net sublimation was 31±21mm, equivalent to 5.1±3.6% of winter snowfall, with a mean daily rate of 0.15 mm/day, placing our estimates at the lower end of previous compilations. During the accumulation period, sublimation accounted for 48% of cumulative winter sublimation and was primarily driven by vapor pressure deficit. In contrast, 52% of cumulative sublimation occurred when the snowpack was melting. For this period, net incoming radiation emerged as the dominant statistical driver of sublimation. Notably, net radiation is only indirectly represented in current energy-balance formulations of physically-based snow models, revealing potential limitations in existing Monin-Obukhov parameterizations. Our results therefore highlight the importance of continuous eddy-covariance observations throughout winter periods for accurately constraining snow sublimation and highlight potential biases in Earth System Models that do not explicitly represent radiative controls on sublimation.

How to cite: Anglin, I., Teuling, R., Floriancic, M., Asemann, P., Lehning, M., and Beria, H.: Magnitude and controls of snow sublimation at a high-elevation Swiss alpine site , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18102, https://doi.org/10.5194/egusphere-egu26-18102, 2026.

EGU26-18457 | ECS | Orals | CR6.8

Changes in Snow Cover from EURO-CORDEX Simulations and Observations: Implications for Surface Energy Budgets and Climate Feedbacks 

Stefanie Börsig, Dominik L. Schumacher, Sven Kotlarski, and Sonia I. Seneviratne

Snow cover strongly influences the surface energy budget, affects seasonal temperature patterns, and shapes regional climate feedbacks. Observation-based estimates indicate that snow–albedo feedbacks can substantially amplify local warming. Yet climate models may underestimate these effects, as limited simulated temperature increases, underestimated snow loss, or mistimed snow melt, particularly in spring and early summer, can dampen the representation of key feedbacks linking snow cover, surface energy fluxes, and near-surface temperature. Such mismatches suggest that important cryosphere–atmosphere interactions may be insufficiently captured in current simulations.

In this study, we link observational datasets and reanalyses with EURO-CORDEX regional climate model simulations to assess how well snow processes are represented across Europe. How well do model-simulated changes in snow amount and seasonality reproduce observed trends in timing and magnitude, and how do differences in snow representation influence surface energy fluxes and near-surface temperatures? By systematically comparing modeled and observed snow-related variables, we aim to identify biases in snow accumulation and melt processes and assess their implications for snow–temperature feedbacks. Addressing these questions is critical for regional climate projections, as underrepresented snow–temperature feedbacks may lead to underestimation of future warming and associated extremes in snow-sensitive regions.

How to cite: Börsig, S., Schumacher, D. L., Kotlarski, S., and Seneviratne, S. I.: Changes in Snow Cover from EURO-CORDEX Simulations and Observations: Implications for Surface Energy Budgets and Climate Feedbacks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18457, https://doi.org/10.5194/egusphere-egu26-18457, 2026.

Western Disturbances (WDs) are upper-tropospheric synoptic-scale systems embedded in the subtropical westerly jet stream, playing a critical role in winter precipitation across the north and northwest Indian subcontinent, including the Himalayas. This study synthesizes insights from multi-decadal analyses (1980–2019) using reanalysis datasets (ERA5, MERRA-2, NCEP-CFSR/CFSv2) to characterize the evolving dynamics, precipitation patterns, and regional impacts of WDs. In the core WD zone of north India, although WD frequency remains relatively stable, a sharp decline (~49%) in intense (strong and extreme) WDs and associated precipitation suggests an increasingly inhibitive dynamic environment with reduced moisture advection. Conversely, over the Karakoram region, WDs have intensified in recent decades, exhibiting a ~10% rise in precipitation intensity and contributing up to ~65% of the total seasonal snowfall. This enhanced snowfall sustains the so-called “Karakoram Anomaly”, a regional glacier stability or mass gain contrasting widespread glacial retreat elsewhere in the Himalayas. The anomaly correlates with declining non-WD snowfall (~17%) and increased baroclinic instability, along with a notable eastward shift (~9.7°E) in the genesis zone of Karakoram WDs toward regions with higher cyclogenesis potential, convergence, and moisture availability. Furthermore, a slowdown in WD propagation speeds has led to more intense and prolonged precipitation events in the region. Collectively, these findings highlight the divergent regional impacts of WDs across the western Himalayas and underscore their central role in driving winter hydroclimate variability, glacier dynamics, and climate change responses in one of the most climate-sensitive regions on Earth.

How to cite: Kumar, P.: Mid-Latitude Dynamical Changes Explain Persistent Glacier Stability in the Karakoram, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18778, https://doi.org/10.5194/egusphere-egu26-18778, 2026.

EGU26-19020 | Posters on site | CR6.8

Linking observations and models to advance knowledge of melting ice in Greenland and Iceland 

Christine S. Hvidberg, Eliza Cook, Guðfinna Aðalgeirsdóttir, and Timothy D. James and the ICELINK team

Record high temperatures have recently been driving significant melting of the Greenland ice sheet, glaciers and permafrost. This ice loss, leading to increased fresh water into the North Atlantic region, risks destabilizing ocean circulation and weather patterns, with severe consequences for local communities in Greenland, Iceland and beyond.

The EU-funded project ICELINK aims to bridge the knowledge gap between climate models, ice-flow models, satellite observations and in-situ observations to accelerate the understanding of how glaciers and ice sheets in the North Atlantic respond to climate change, and their impacts on climate and ecosystems. Through improved understanding of snow, surface mass balance and the ice dynamical response to meltwater runoff, ICELINK will provide new knowledge of the processes that control the evolution of the Greenland ice sheet and Icelandic glaciers in response to global warming. Specifically, ICELINK will work with local communities to co-develop knowledge and strengthen adaptation strategies, helping them to mitigate risks and build resilience on hydrology and ecosystem risks. Further, ICELINK will use Icelandic glaciers as a data-observation laboratory to study the response of the Greenland ice sheet in a warmer world with more melting.

The presentation will discuss the importance of including observation-based knowledge to understand the mass loss from the Greenland ice sheet and Icelandic glaciers, which is a key focus of ICELINK. We will give an update on our research towards obtaining consistent observations-and-model-integrated datasets on surface mass balance (SMB), the ice dynamical response to surface melt and historical records of climate forcing trends and variability. These are key components in understanding the melting of North Atlantic ice and assessing the impact on Earth’s climate.

How to cite: Hvidberg, C. S., Cook, E., Aðalgeirsdóttir, G., and James, T. D. and the ICELINK team: Linking observations and models to advance knowledge of melting ice in Greenland and Iceland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19020, https://doi.org/10.5194/egusphere-egu26-19020, 2026.

EGU26-20800 | Posters on site | CR6.8

The onset of a surge in Dyngjujökull outlet glacier in N-Vatnajökull, Iceland 

Finnur Pálsson, Eyjólfur Magnússon, Vincent Drouin, Thomas Nagler, Valentyn Tolpekin, Joaquín M.C. Belart, Jan Wuite, Hrafnhildur Hannesdóttir, Tómas Jóhannesson, Birgir V. Óskarsson, and Andri Gunnarsson

Dyngjujökull is a surge-type outlet glacier, which in 2025 covered ~1030 km2, corresponding to more than 1/8 of Vatnajökull ice cap. Dyngjujökull has a surge interval of 20–30 years with the last surge occurring in 1998–2000. During that surge, ~12 km3 of ice was transported from Dyngjujökull’s reservoir area to the receiving area and the glacier margin advanced by ~2 km. The motion of Dyngjujökull has been measured at mass-balance stakes near its centre flow line since 1993. In spring 2025, a GNSS station was deployed at stake location D7, at elevation 1350 m a.s.l., slightly above the glacier equilibrium line. The velocity at this site had in recent years been gradually increasing from 60 to 90 m a–1 repeating similar development as observed prior to the last surge. The measured average velocity at D7 in the summer 2025 was 150 m a–1, approximately the same as observed at the start of the last surge in summer 1998, strongly indicating the onset of a new surge. Here we will present the evolution of ice motion of Dyngjujökull at the start of this surge, in winter 2025–26, extracted from multiple radar satellites, including ICEYE, Sentinel-1, TerraSAR-X/TanDEM-X and SAOCOM, and GNSS stations operated on the glacier. We also aim to present elevation changes deduced from Pléiades satellite DEMs planned for February to April, 2026.

How to cite: Pálsson, F., Magnússon, E., Drouin, V., Nagler, T., Tolpekin, V., Belart, J. M. C., Wuite, J., Hannesdóttir, H., Jóhannesson, T., Óskarsson, B. V., and Gunnarsson, A.: The onset of a surge in Dyngjujökull outlet glacier in N-Vatnajökull, Iceland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20800, https://doi.org/10.5194/egusphere-egu26-20800, 2026.

EGU26-21280 | Orals | CR6.8

Changes in permafrost distribution in the Hornsund Area (Svalbard) based on ERT surveys from 2010 - 2025 

Marta Kondracka, Szymon Oryński, Dariusz Ignatiuk, Marek Kasprzak, Krzysztof Senderak, and Maurycy Kot

Rapid changes in the cryosphere, including permafrost, glaciers, and snow cover, are increasingly altering polar environments, with significant implications for climate feedbacks, hydrology, ecosystem functioning, and biogeochemical cycles. In polar regions, these transformations are particularly pronounced in post-glacial landscapes, where surface and subsurface processes respond sensitively to ongoing climatic forcing.

This study presents the results of long-term investigations of permafrost distribution and degradation in the Hornsund area (Svalbard), based on electrical resistivity tomography (ERT) surveys conducted between 2010 and 2025. Geophysical measurements were carried out across a range of geomorphological settings, including marine terraces, mountain slopes, coastal zones, and the forefields of retreating glaciers. The multi-site and multi-temporal ERT dataset enabled detailed identification and characterization of permafrost occurrence, thickness, and internal structure under varying environmental conditions.

The 15-year observation period provides a robust basis for assessing spatio-temporal changes in permafrost distribution and for identifying signs of progressive degradation in selected areas. Observed resistivity patterns indicate a reduction in permafrost continuity and thickness. These results contribute to improved quantification of the impacts of permafrost change on hydrological regimes, sediment and nutrient transport, coastal stability, and ecosystem dynamics. The findings highlight the importance of long-term geophysical monitoring in reducing uncertainties associated with projections of cryosphere climate interactions and their broader environmental consequences.

 

How to cite: Kondracka, M., Oryński, S., Ignatiuk, D., Kasprzak, M., Senderak, K., and Kot, M.: Changes in permafrost distribution in the Hornsund Area (Svalbard) based on ERT surveys from 2010 - 2025, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21280, https://doi.org/10.5194/egusphere-egu26-21280, 2026.

EGU26-21397 | ECS | Posters on site | CR6.8

Subsurface ice interpretation using joint seismic-electrical responses and rock physics diagnostic 

Ary Leonel Miño and Michele Pipan

The detection of liquid water and ice, as well as the discrimination between frozen and unfrozen geological materials, remains a major challenge in periglacial geophysics. Seismic refraction and electrical resistivity tomography are widely applied to address this problem (Hauck et al., 2011; Mollaret et al., 2020); however, similar velocity and resistivity anomalies may originate from distinct physical configurations, including pore-filling ice, massive ice bodies, or heterogeneous mixtures of frozen and unfrozen materials. This intrinsic non-uniqueness complicates the interpretation of field geophysical data and limits the ability to infer the elastic contribution of ice to the seismic response. 

In this study, we investigate how the assumed physical behaviour and spatial distribution of ice influence the joint interpretation of seismic velocity and electrical resistivity responses. Field geophysical datasets are analysed using a phase-based petrophysical joint inversion framework that estimates volumetric fractions of liquid water, ice, air, and solid matrix by coupling seismic refraction velocities and electrical resistivity following four-phases model scheme (Wagner et al., 2019). The seismic forward response is governed by effective-medium rock-physics formulations that explicitly account for the elastic contribution of ice (Mavko et al., 2009), whereas electrical resistivity is primarily controlled by the connected liquid water phase under Archie-type assumptions (Archie, 1942).To support the interpretation of the field inversion results, a suite of synthetic models is constructed to represent end-member and transitional ice configurations, including pore-filling ice, massive ice, and patchy distributions of ice-bearing and ice-free domains. Ice-related elastic properties are modelled using self-consistent approximation (SCA) effective-medium theory (Mavko et al., 2009), while electrical properties remain dominated by liquid water content following Archie-type relationships (Archie, 1942). Synthetic seismic and electrical datasets are generated and inverted using the same workflow applied to the field data, providing physically consistent reference scenarios for interpretation. 

Comparison between synthetic and field inversion results reveals systematic differences in the coupled seismic–electrical response associated with volumetric ice contributions versus elastically stiff ice contributions to the seismic response. While multiple ice configurations may reproduce either seismic velocity increases or resistivity anomalies independently (Hauck et al., 2011), only a limited subset of scenarios yields mutually consistent fits to both datasets when rock-physics constraints are considered. Mismatches between inferred phase fractions, seismic velocity enhancement, and resistivity contrasts serve as diagnostic indicators for rejecting physically implausible interpretations and avoiding interpretational pitfalls. 

Although a unique determination of ice type is not achievable, the combined use of rock-physics-informed joint inversion and synthetic reference models significantly reduces interpretational ambiguity. The results highlight the value of physically constrained joint inversion as a diagnostic tool for assessing the presence and elastic relevance of subsurface ice in periglacial environments. 

How to cite: Miño, A. L. and Pipan, M.: Subsurface ice interpretation using joint seismic-electrical responses and rock physics diagnostic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21397, https://doi.org/10.5194/egusphere-egu26-21397, 2026.

EGU26-211 | ECS | Orals | SM3.4

Automatic detection and classification of Nanoseismicity in Distributed Acoustic Sensing data 

Dominic Seager, Jessica Johnson, Lidong Bie, Beatriz De La Iglesia, and Ben Milner

The detection of nanoseismicity (very tiny earthquakes sometimes associated with small cracks in rock, also called acoustic emissions) is an important area of research aiding in the understanding of geophysical processes, hazard detection, material failure and human-driven nanoseismicity. The high frequency and attenuation of nanoseismicity require high-frequency monitoring within metres of the source to capture the event. This has made them difficult to monitor in conditions outside of small-scale lab experiments, in which failure is intentionally induced. The development of distributed acoustic sensing (DAS) as a new tool for seismic monitoring, however, has increased the feasibility of investigating such signals in the field due to its high temporal and spatial resolution. Manual picking of these events, while possible, is impractical for long-term deployments and for time-critical applications such as stability monitoring, which limits the utility of the technology. Automation of the detection of nanoseismic events within such data is therefore essential for the long-term processing of DAS data and real-time processing of data for use in stability monitoring.  

We have developed a pipeline for the automated extraction of nanoseismic events from DAS data, using a new, simple ratio technique called Spatial Short-Term Average (SSTA). The pipeline takes an input of DAS data and generates a series of windows within the data containing information about high amplitude signals relating to nanoseismicity.  

Using the automatically detected events, we labelled the windows to train a series of machine learning models to classify the different signals. Once trained, we evaluated the performance of the various models to select the most effective method for processing the collected data. The best performing models will then be tested at scale with the resulting classified dataset being plotted spatially along the length of the deployment to identify patterns of activity across space and time. 

How to cite: Seager, D., Johnson, J., Bie, L., De La Iglesia, B., and Milner, B.: Automatic detection and classification of Nanoseismicity in Distributed Acoustic Sensing data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-211, https://doi.org/10.5194/egusphere-egu26-211, 2026.

EGU26-893 | ECS | Orals | SM3.4

Optical Interferometry-based seafloor cable Measurements for Rupture Imaging and Tsunami Signal Analysis in the Southwest Pacific 

Amin A. Naeini, Bill Fry, Giuseppe Marra, Max Tamussino, Johan Grand, Jennifer D. Eccles, Kasper van Wijk, Dean Veverka, and Ratnesh Pandit

Optical interferometry on submarine fiber-optic telecommunication cables offers a transformative opportunity for offshore geohazard monitoring by providing continuous measurements of seafloor perturbation at useful intervals over trans-oceanic distances (Marra et al., 2022). We analyze a southwest Pacific subset of data from a section of the Southern Cross NEXT cable connecting Auckland (New Zealand) to Alexandria (Australia). Using only cable-based measurements, we image the seismic rupture kinematics of the 17 December 2024 Mw 7.3 Vanuatu earthquake, the largest seismic event recorded on this cable since its installation.

 

We analyze measurements of a section of cable more than 1,000 km in length and comprising 18 inter-repeater spans including the section that runs roughly parallel to the Vanuatu subduction zone and the adjoining section extending southward toward New Zealand. The earthquake produces clear and coherent arrivals in the optical frequency deviation recorded across multiple spans, with well-defined signatures visible in both time series and spectrograms. We first extract earthquake-related strain signals in the 0.1-0.3 Hz frequency band and apply the Multiple Signal Classification (MUSIC) back-projection technique to recover the source-time evolution of the rupture. The inferred rupture is predominantly bilateral and consistent with the USGS finite-fault solution, confirming that interferometric submarine cables can function as effective regional seismic arrays for rapid characterization of offshore earthquakes.

 

These results further demonstrate the capability of submarine fiber-optic cables to image earthquake rupture processes using high-frequency strain signals, providing valuable monitoring coverage, especially in instrumentally sparse regions such as the southwest Pacific. By resolving rupture kinematics directly, cable-based observations offer a pathway toward improved tsunami early-warning strategies that rely less on empirical magnitude–scaling relations, which are uncertain for large earthquakes. Planned upgrades of the interrogating laser will allow the performance of this approach to be assessed at lower frequencies, where cable-based observations may provide direct constraints on tsunami propagation and other long-period geophysical processes.

How to cite: A. Naeini, A., Fry, B., Marra, G., Tamussino, M., Grand, J., D. Eccles, J., van Wijk, K., Veverka, D., and Pandit, R.: Optical Interferometry-based seafloor cable Measurements for Rupture Imaging and Tsunami Signal Analysis in the Southwest Pacific, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-893, https://doi.org/10.5194/egusphere-egu26-893, 2026.

EGU26-1594 | ECS | Orals | SM3.4

Physics-based earthquake early warning using distributed acoustic sensing 

Itzhak Lior and Shahar Ben Zeev

We present a physics-based point source earthquake early warning system using distributed acoustic sensing (DAS) data. All core modules of the system are based on physical principles of wave propagation, and models that describe the earthquake source and far-field ground motion. The detection-location algorithm is based on time-domain delay-and-sum beamforming, and the magnitude estimation and ground motion prediction are performed using analytical equations based on the Brune omega squared model. We demonstrate the performance of the system in terms of magnitude estimation and ground motion prediction, and in terms of real-time computational feasibility using local 3.1 ≤ M ≤ 3.6 earthquakes. This DAS early warning system allows for fast deployment, circumventing some calibration phases that require gathering local DAS earthquake data before the system becomes operational.

How to cite: Lior, I. and Ben Zeev, S.: Physics-based earthquake early warning using distributed acoustic sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1594, https://doi.org/10.5194/egusphere-egu26-1594, 2026.

EGU26-3915 | ECS | Orals | SM3.4

Quasi-static waveform inversion from DAS observations 

Le Tang, Etienne Bertrand, Eléonore Stutzmann, Luis Fabian Bonilla Hidalgo, Shoaib Ayjaz Mohammed, Céline Gélis, Sebastien Hok, Maximilien Lehujeur, Donatienne Leparoux, Gautier Gugole, and Olivier Durand

As a vehicle approaches the fiber-optic cable, the distributed acoustic sensing (DAS) records a broadband strain rate, which corresponds to propagating seismic waves at high frequencies (>1Hz) and to quasi-static strain fields at low frequencies (<1Hz). However, characterizing the subsurface media through quasi-static deformations remains challenging. Here, we propose a new method for imaging shallow urban subsurface structures using quasi-static strain waveforms, measured with fiber-optic cables. This technique utilizes the quasi-static waveform of a single DAS channel to generate a local 1D velocity model, thereby enabling high-resolution imaging of the underground using thousands of densely packed channels. We employed the Markov Chain Monte Carlo (MCMC) inversion strategy to investigate the depth range of inversion using car-induced quasi-static waveforms. The synthetic data demonstrates that the quasi-static strain field generated by a standard small car moving over the ground enables detailed imaging of structures at depths from 0 to 10 meters. Additionally, we conducted field experiments to measure the 2D shear-wave velocity model along a highway using quasi-static strain waveforms generated by a four-wheeled small car. The velocity structure we obtained is closely aligned with that derived from the classical surface-wave phase-velocity inversion. This consistency indicates that the inversion depth range is comparable to the simulation results, which confirms the applicability of this method to real data. In the future, we anticipate using the city's extensive fiber-optic communication network to record quasi-static deformations induced by various types of vehicles, thereby enabling imaging of the urban subsurface at a citywide scale. This will provide valuable insights for the design of urban underground infrastructure and for assessing urban hazards and risks.

How to cite: Tang, L., Bertrand, E., Stutzmann, E., Bonilla Hidalgo, L. F., Mohammed, S. A., Gélis, C., Hok, S., Lehujeur, M., Leparoux, D., Gugole, G., and Durand, O.: Quasi-static waveform inversion from DAS observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3915, https://doi.org/10.5194/egusphere-egu26-3915, 2026.

EGU26-4163 | Orals | SM3.4

Seismic data telemetry system and precise hypocenter location for distributed acoustic sensing observation using seafloor cable off Sanriku, Japan 

Masanao Shinohara, Shun Fukushima, Kenji Uehira, Youichi Asano, Shinichi S. Tanaka, and Hironori Otsuka

A seismic observation using Distributed Acoustic Sensing (DAS) using seafloor cable can provide spatially high-density data for a long distance in marine areas. A seafloor seismic and tsunami observation system using an optical fiber cable off Sanriku, northeastern Japan was deployed in 1996. Short-term DAS measurements were sporadically repeated since February 2019 using spare fibers of the Sanriku system (Shinohara et al., 2022). A total measurement length is approximately 100 km.  It has been concluded that measurement with a sampling frequency of 100 Hz, a ping rate of 500 Hz, gauge length of 100 m, and a spatial interval of 10 m is adequate for earthquake and tsunami observation.  From March 2025, we started a continuous DAS observation to observe seismic activity. When the continuous DAS observation was commenced, we developed quasi real time data transmission system through the internet. Because a DAS measurement generates a huge mount of data per unit time and capacity of internet is limited, decimation for spatial direction is adopted. In addition, data format is converted from HDF5 to conventional seismic data exchange format in Japan (win format). An interrogator generates a HDF5 file every 30 seconds. After the file generation, the telemetry system reads the HDF5 file, and decimates data for spatial domain. Then, the data format is changed to the win format and the data are sent to the internet. In other words, data transmission is delayed for a slightly greater than 30 seconds. Data with the win format can be applied to various seismic data processing which has been developed before. To locate a hypocenter using DAS data, seismic phases in DAS data must be identified. To evaluate performance of hypocenter location using DAS records, arrival times of P- and S-waves were picked up on the computer display for local earthquakes. Every 100 channel records on DAS data and data from surrounding ordinary seismic stations were used. Location program with absolute travel times and one-dimensional P-wave velocity structure was applied. Results of location of earthquakes were evaluated by mainly using location errors. Errors of the location with DAS data were smaller than those of the location without the DAS data. Increase of arrival data for DAS records seems to be efficient to improve a resolution. However, picking up signals for all channels (seismic station) manually are costly due to a large number of channels. To expand the location method, an improved automatic pick-up program using evaluation function from conventional seismic network data by seismometers for DAS data (Horiuchi et al., 2025) was applied to the DAS data obtained by the Sanriku system. As a result, arrivals time of P, S and converted PS waves can be precisely identified with high resolution. We have a plan to locate earthquakes using all DAS channels (seismic stations)  and surrounding ordinary marine and land seismic stations.

How to cite: Shinohara, M., Fukushima, S., Uehira, K., Asano, Y., Tanaka, S. S., and Otsuka, H.: Seismic data telemetry system and precise hypocenter location for distributed acoustic sensing observation using seafloor cable off Sanriku, Japan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4163, https://doi.org/10.5194/egusphere-egu26-4163, 2026.

EGU26-4254 | Orals | SM3.4

Using a hybrid seismic and Distributed Acoustic Sensing (DAS) network to study microseismicity in high spatiotemporal resolution offshore of Kefalonia Island, Greece  

Rebecca M. Harrington, Gian Maria Bocchini, Emanuele Bozzi, Marco P. Roth, Sonja Gaviano, Giulio Pascucci, Francesco Grigoli, Ettore Biondi, and Efthimios Sokos

Combining traditional seismic networks with Distributed Acoustic Sensing (DAS) to record ground-motion on telecommunications cables provides new opportunities to study small earthquakes with unprecedented spatial and temporal resolution. Here we present a detailed study of an earthquake sequence offshore northwest of Kefalonia island, Greece that began in March 2024 and returned to background levels by November–December. The sequence was recorded by both a permanent seismic network for its duration and by DAS on a fiber-optic telecommunications cable between 1 - 15 August 2024.  The two-week DAS dataset provides continuous strain measurements along ~15 km of optical fiber between northern Kefalonia and Ithaki during a period that captured elevated seismic activity. Combining seismic station and DAS data reveals distinct physical features of the sequence that are not observable with seismic stations alone, including details of mainshock-aftershock clustering and well-resolved source spectra at frequencies of up to ~50 Hz for M < 3 events. The signal-to-noise-ratio > 3 at frequencies of up to 50 Hz observed on DAS waveforms for a representative group of events suggests consistency with typical earthquake stress-drop values that range from 1-10 MPa. It further suggests that DAS data may be used to augment detailed studies of microearthquake source parameters.

We apply semblance-based detection to DAS waveforms and manually inspect 5,734 earthquakes that occurred within ~50 km of the fiber to build an initial earthquake catalog. We then combine DAS and seismic-station data to locate 284 events with high signal-to-noise ratios and compute their local magnitudes with seismic station data to create a detailed subset of the initial catalog. We apply waveform cross-correlation to offshore DAS data for events in the detailed catalog to associate unlocated detections with template events and estimate relative magnitudes from amplitude ratios and further enhance the detailed catalog. This approach adds an additional 2,496 earthquakes (2,780 events in total) with assigned locations and magnitudes and leads to an enhanced catalog with completeness magnitude Mc = -0.5. Most earthquakes (2,718 of 2780) cluster within a ~5 km radius approximately 10 km offshore of northwestern Kefalonia and exhibit local rates exceeding 100 events per hour.

Our enhanced catalog provides a detailed spatiotemporal record of seismicity in a region with limited station coverage and demonstrates the effectiveness of integrating DAS with seismic networks for earthquake monitoring of active seismic sequences. Furthermore, it resolves details of mainshock–aftershock clustering that would have otherwise likely have been erroneously classified as swarm-like with standard monitoring, highlighting how observational resolution influences the interpretation of the physics driving earthquake sequences.

How to cite: Harrington, R. M., Bocchini, G. M., Bozzi, E., Roth, M. P., Gaviano, S., Pascucci, G., Grigoli, F., Biondi, E., and Sokos, E.: Using a hybrid seismic and Distributed Acoustic Sensing (DAS) network to study microseismicity in high spatiotemporal resolution offshore of Kefalonia Island, Greece , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4254, https://doi.org/10.5194/egusphere-egu26-4254, 2026.

The first commercially available fibre-optic Distributed Acoustic Sensing (DAS) system, Cobolt, was released in 2004, with early uptake driven by applications in perimeter security, pipeline monitoring, and upstream oil and gas operations. Although these deployments demonstrated the disruptive potential of DAS, it is only within the past five years that the geoscience community has widely embraced the technology, exploiting its ability to deliver continuous, high-fidelity measurements with exceptional spatial and temporal resolution.

Historically, commercially available DAS systems were optimised for industrial monitoring rather than scientific metrology. As a result, key requirements of geoscience applications—such as quantitative accuracy, extreme sensitivity, extended range, and robustness in challenging environments—were not primary design drivers. This situation is now changing rapidly as geoscience applications mature and expand. This contribution reviews the principal performance characteristics that define the suitability of modern DAS systems for geoscience research and examines how recent technological developments are addressing these needs.

Five performance parameters are of particular importance. First, the transition from amplitude-based, qualitative DAS to phase-based, quantitative systems has enabled true strain-rate and strain measurements suitable for metrological applications. Second, instrument sensitivity has improved by several orders of magnitude, with contemporary systems achieving pico-strain-level detection along standard telecom fibre. Third, measurement range—ultimately limited by available backscattered photons in pulsed DAS—has been extended beyond 150 km through the adoption of spread-spectrum interrogation techniques. Fourth, spatial resolution continues to improve, with gauge lengths of ≤1 m and sampling intervals of ≤0.5 m now routinely achievable, and further reductions anticipated. Finally, dynamic range remains a critical consideration for high-amplitude signals such as earthquakes; however, reductions in gauge length provide a clear pathway to mitigating cycle-skipping limitations, supporting the future use of DAS in Earthquake Early Warning (EEW) systems.

Alongside raw performance, the ability to quantify and compare DAS system capabilities has become increasingly important. Industry-led efforts have resulted in well-defined test methodologies and performance metrics, providing a common framework for objective evaluation of DAS instruments used in scientific studies.

Practical deployment considerations are also shaping system design. Reduced size, weight, and power (SWaP) enable operation in remote and hostile environments, while improved reliability, passive cooling, and environmental sealing facilitate long-term field installations. These advances are particularly relevant to emerging marine and subsea applications, where low-power, marinised DAS systems are required for seabed deployment.

Finally, the growing complexity of DAS instrumentation places increasing emphasis on software. Automated configuration, intuitive user interfaces, and integrated edge-processing capabilities are becoming essential to ensure that non-specialist users can reliably extract high-quality scientific data.

Together, these developments signal a transition in DAS from an industrial monitoring tool to a mature geoscience instrument, with continued innovation expected to further expand its role across solid-Earth, cryospheric, and marine research over the coming decade.

How to cite: Hill, D.: DAS design features critical to geoscience applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4295, https://doi.org/10.5194/egusphere-egu26-4295, 2026.

EGU26-4413 | ECS | Posters on site | SM3.4

Coherent Source Subsampling of Seismic Noise for Distributed Acoustic Sensing in the Swiss Alps 

Sanket Bajad, Daniel Bowden, Pawan Bharadwaj, Elliot James Fern, Andreas Fichtner, and Pascal Edme

Distributed Acoustic Sensing (DAS) provides dense measurements of seismic noise along fiber-optic cables and offers new opportunities for subsurface characterization. In environments where controlled sources are unavailable, conventional noise interferometry workflows for DAS construct virtual shot gathers via cross-correlation and average them over long time windows to obtain coherent surface waves for dispersion analysis and subsequent shear-wave velocity (Vs) inversion. In noise-based interferometric imaging, the distribution of noise sources controls the quality of the retrieved interstation response. In practice, seismic sources are highly anisotropic and intermittent, and so simply averaging all available time windows produces interferometric responses that are difficult to interpret and lead to unstable dispersion curves and biased Vs estimates. We present a data-driven coherent source subsampling (CSS) framework that automatically identifies and selects the time windows of seismic noise that contribute constructively to the physically interpretable interstation response.

We demonstrate the method using DAS data acquired along 30 km of pre-existing telecommunication fiber deployed by the Swiss Federal Railways (SBB) in a major alpine valley floor, recorded with a Sintela interrogator at 3 m channel spacing with 6 m gauge length. Our objective is to recover stable Rayleigh-wave dispersion curves and a shallow Vs structure in the upper 50 m. The fiber runs along the railway track in surface cable ducts, providing a realistic test bed with complex ambient noise, including car traffic, factories, quarry blasts, in addition to the train-generated signals. Subsampling strategies based on prior knowledge of the sources, such as train schedules or velocity-based filtering, can partly mitigate this problem. However, these strategies are tedious, strongly location-dependent along the fiber, and do not guarantee that the retained windows contribute coherently to the interstation response of the segment under investigation.

Here, we use a symmetric variational autoencoder (SymVAE) to perform coherent source subsampling. Trained on virtual shot gathers from multiple time windows, the SymVAE groups windows according to the similarity of their correlation wavefields and enables the selection of those windows that consistently exhibit symmetric surface-wave contributions on both the causal and acausal sides. Averaging only these subsampled windows yields interstation responses that are substantially denoised and symmetric. We interpret these cleaner and symmetric cross-correlations as being associated with the stationary-phase contributions for the fiber segment under investigation. The same framework also identifies fiber segments that lack coherent, dispersive Rayleigh waves, indicating where robust subsurface imaging is not feasible.

Applying CSS to the SBB DAS data produces stable Rayleigh-wave dispersion curves along the cable, which we invert for two-dimensional Vs profiles. Although demonstrated here on railway-generated noise, the proposed CSS framework can be extended to any uncontrolled settings, such as road-traffic-dominated areas, where source variability and non-uniformity may be even more severe.

  • 1Centre for Earth Sciences, Indian Institute of Science, Bangalore, India
  • 2Department of Earth and Planetary Sciences, ETH Zurich, 8092 Zurich, Switzerland
  • 3 SBB CFF FFS

 

How to cite: Bajad, S., Bowden, D., Bharadwaj, P., Fern, E. J., Fichtner, A., and Edme, P.: Coherent Source Subsampling of Seismic Noise for Distributed Acoustic Sensing in the Swiss Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4413, https://doi.org/10.5194/egusphere-egu26-4413, 2026.

EGU26-4603 | ECS | Orals | SM3.4

What Controls Variability in DAS Earthquake Observations? Implications for Ground-Motion Models 

Chen-Ray Lin, Sebastian von Specht, and Fabrice Cotton

Distributed Acoustic Sensing (DAS) provides dense, meter-scale ground-motion measurements along fiber-optic cables. However, developing ground-motion models (GMMs) from DAS data is challenging because observations are controlled by DAS-specific factors such as cable coupling, orientation, and channel correlation. In this study, we present the first regional, partially non-ergodic DAS-based GMM that explicitly identifies and quantifies cable-related contributions to ground-motion variability. We analyze strain-rate data from a 400-channel DAS array at the Milun campus in Hualien City, Taiwan, compiling peak strain rates and Fourier amplitudes (0.1–10 Hz) from 77 regional earthquakes (3<M<7, 45<R<170 km). Building on classical seismometer-based GMMs, we extend the variability framework to account for (1) cable coupling influenced by installation and environment types, (2) cable orientation, and (3) channel correlation inherent to DAS measurement principles and array geometry. Channel correlation is modeled using Matérn kernels parameterized by along-fiber and spatial proximity distances. The resulting DAS-based GMM shows magnitude-distance scaling comparable to classical models, while decomposing variability into physically interpretable components. Cable coupling emerges as a dominant broadband source of within-event variability, whereas orientation effects capture repeatable, frequency-dependent earthquake source radiation patterns. Modeling channel correlation significantly reduces channel-related standard deviations, demonstrating that treating DAS channels as independent observations biases uncertainty estimates. Overall, our results show that DAS-derived ground motions require a fundamentally different variability framework than that of classical GMMs, highlighting the importance of deployment metadata and correlation modeling. This approach provides a statistical and physical foundation for next-generation seismic hazard assessments using dense fiber-optic sensing.

How to cite: Lin, C.-R., von Specht, S., and Cotton, F.: What Controls Variability in DAS Earthquake Observations? Implications for Ground-Motion Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4603, https://doi.org/10.5194/egusphere-egu26-4603, 2026.

Monitoring fin whale (Balaenoptera physalus) vocalizations is of significant scientific importance and practical value for marine ecology, hydroacoustics, and geophysics. Conventional monitoring approaches, such as hydrophone arrays, ocean-bottom seismometers (OBS), and satellite tagging, are limited by sparse spatial coverage, potential biological disturbance, and high costs. Distributed acoustic sensing (DAS) is an emerging technology that utilizes submarine optical cables as dense acoustic arrays, providing opportunities for large-scale, high-resolution monitoring of whale vocalizations. Here, we reveal the wavefield features of fin whale vocalizations by integrating DAS observational data combined with numerical simulations. Three distinct features—Insensitive response segment (IRS), high-frequency component loss, and acoustic notch—were identified in the observed wavefield. DAS response analysis via ray-acoustic modeling indicates that the length of the IRS is positively correlated with the vertical source-to-cable distance, while the gauge length is responsible for the high-frequency loss in Type-B calls. Furthermore, wavefield simulations using the spectral-element method (SEM) demonstrate that the acoustic notches represent transitions between transmission zones of waterborne multipath waves entering the seafloor, exhibiting high sensitivity to the seafloor P-wave velocity, water depth, and topography. These findings not only enhance our understanding of the DAS-observed wavefields, but also highlight the potential of utilizing DAS and acoustic notches for ocean environmental parameter estimation.

How to cite: Wang, Q.: Revealing the Wavefield Features of Fin Whale Vocalizations Observed by Distributed Acoustic Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4625, https://doi.org/10.5194/egusphere-egu26-4625, 2026.

This study aims to develop a system for the identification of vessels, seismic events, and volcanic activity through analysis of the spatiotemporal characteristics of wavefields recorded by distributed acoustic sensing (DAS) using a submarine fiber-optic cable. DAS provides unprecedented spatial coverage and resolution, making it highly suitable for monitoring dense wavefield variations and anthropogenic activities, whereas traditional seismometers remain indispensable for quantitative seismic analysis and low-frequency observations. In this study, continuous DAS records acquired from a submarine fiber-optic cable located in the northeastern offshore region of Taiwan near Guishan Island, an active volcano. This region experiences frequent seismic activity due to the northwestward subduction of the Philippine Sea Plate beneath the Eurasian Plate. In addition, the passage of the Kuroshio Current, a warm ocean current, brings abundant fish resources, resulting in frequent activities of fishing vessels and whale-watching boats. Event detection is first carried out using the recursive short-time-average/long-time-average (STA/LTA) method which uses two time windows with different durations and computes the average signal amplitude within each window. When a signal arrives, the average amplitude within a short time window changes rapidly, thereby increasing the ratio of the short-time average to the long-time average. An event is detected when this ratio exceeds a predefined threshold and manual secondary inspected. However, low signal-to-noise ratios (SNR) can significantly reduce the sensitivity of STA/LTA-based detection, leading to missed events. To overcome this problem, signal processing adjustments were applied to enhance detection performance. To validate the detection performance, the detected ship-related events were compared with records from the Automatic Identification System (AIS), while earthquake events identified from the DAS data were compared with the earthquake catalog of Taiwan Seismological and Geophysical Data Management System (GDMS). Subsequently, a regression analysis of catalog magnitudes against hypocentral distance and maximum DAS-recorded amplitude was applied to determine the minimum detectable earthquake magnitude. The proposed framework demonstrates the potential of DAS as a complementary tool for offshore geophysical and maritime monitoring, providing a basis for future studies on vessel tracking, seafloor topography, and earthquake monitoring.

How to cite: Wei, Y. J. and Chan, C. H.: Application of Distributed Acoustic Sensing to Detect and Identify of Vessels and Natural Events in the Northeastern Offshore Region of Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4712, https://doi.org/10.5194/egusphere-egu26-4712, 2026.

EGU26-5156 * | Orals | SM3.4 | Highlight

Englacial ice quake cascades in the Northeast Greenland Ice Stream - Observations and implications of ice stream dynamics 

Andreas Fichtner, Coen Hofstede, Brian Kennett, Anders Svensson, Julien Westhoff, Fabian Walter, Jean-Paul Ampuero, Eliza Cook, Dimitri Zigone, Daniela Jansen, and Olaf Eisen

Ice streams are major contributors to ice sheet mass loss and critical regulators of sea level change. Despite their important, standard viscous flow simulations of ice stream deformation and evolution have limited predictive power, mostly because our understanding of the involved processes is limited. This leads, for instance, to widely varying predictions of sea level rise during the next decades.

 

Here we report on a Distributed Acoustic Sensing experiment conducted in the borehole of the East Greenland Ice Core Project (EastGRIP) on the Northeast Greenland Ice Stream. For the first time, our observations reveal a brittle deformation mode that is incompatible with viscous flow over length scales similar to the resolution of modern ice sheet models: englacial ice quake cascades that are not being recorded at the surface. A comparison with ice core analyses shows that ice quakes preferentially nucleate near volcanism-related impurities, such as thin layers of tephra or sulfate anomalies. These are likely to promote grain boundary cracking, and appear as a macroscopic form of crystal-scale wild plasticity. A conservative estimate indicates that seismic cascades are likely to produce strain rates that are comparable in amplitude to those measured geodetically, thereby bridging the well-documented gap between current ice sheet models and observations.

How to cite: Fichtner, A., Hofstede, C., Kennett, B., Svensson, A., Westhoff, J., Walter, F., Ampuero, J.-P., Cook, E., Zigone, D., Jansen, D., and Eisen, O.: Englacial ice quake cascades in the Northeast Greenland Ice Stream - Observations and implications of ice stream dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5156, https://doi.org/10.5194/egusphere-egu26-5156, 2026.

We present a back-projection based earthquake location method tailored to Distributed Acoustic Sensing (DAS) arrays, using short overlapping fiber segments and a combined P–S framework to reliably locate local earthquakes. A 66km quasi-linear telecommunication fiber in Israel was repurposed as a DAS array. We analyzed several local earthquakes with varying source–array geometries. We divided the fiber into overlapping 5.4 km segments and back-projected P- and S-wave strain-rate recordings using a local 1D velocity model over a regional grid of potential earthquake locations. Each grid point is assigned with P- and S-phase semblance, and the corresponding phase-specific origin times, associated with the timing of maximum semblance. Segment-specific P- and S-phase semblance maps and the difference between P and S origin times were combined through a weighting scheme that favors segments with spatially compact high-semblance regions. The objective is maximizing both P- and S-wave semblance and minimizing P- and S-wave origin time discrepancies. Results for the analyzed earthquakes reveal robust constraints on both azimuth and epicentral distance from the fiber, and demonstrate the ability to mitigate DAS-related artifacts associated with broadside sensitivity and reduced coherency. We demonstrated the potential of the approach for real-time earthquake location and showed its performance when only P-wave recordings are available, underscoring the method’s potential for future DAS-based earthquake early warning implementation.

How to cite: Noy, G., Ben Zeev, S., and Lior, I.: Earthquake Location using Back Projection with Distributed Acoustic Sensing with Implications for Earthquake Early Warning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5259, https://doi.org/10.5194/egusphere-egu26-5259, 2026.

EGU26-5274 | ECS | Orals | SM3.4

Spectral analysis of background and transient signals at Mount Etna using rectilinear fibre-optic segments 

Hugo Latorre, Sergio Diaz-Meza, Philippe Jousset, Sergi Ventosa, Arantza Ugalde, Gilda Currenti, and Rafael Bartolomé

Etna is the largest, most active and closely monitored volcano in Europe,
making it a crucial study region for volcanology and geohazard assessment. In early
July 2019, a 1.5 km fibre-optic cable was deployed near the summit of Mount Etna
and interrogated for two months. The cable was divided into four main segments, two
of which point towards different active crater areas. Temporary seismic broadband
stations and infrasound sensors were also deployed along the cable. During the
experiment, three distinct eruptive events were recorded. The first two events are
characterised by a large number of explosions in the active crater area, together with
an increase in background tremor activity. The third event is characterised by a larger
increase in background tremor, but almost no explosions.

The continuous recordings are analysed in the frequency-wavenumber domain,
which reveals the features of the background tremor activity and the stacked transient
signals, such as explosions. During the first two eruptive events, the stack of
explosive sources is characterised by a non-dispersive arrival, travelling with
different apparent velocities along each segment, and a non-linear ground response up
to 25 Hz. These segments can be used as an antenna to estimate an average back-
azimuth for the explosions, which come from the same crater area during both
eruptive events.

Outside of the three eruptive events, the background tremor features two slow
dispersion modes, both well resolved on the raw recordings. The slowest mode is
affected by gauge-length attenuation at higher frequencies, due to its short
wavelength, but remains detectable up to 27 Hz, with group velocities as low as 170
m/s. These observations showcase the utility of simple, rectilinear geometries in
deployments despite their known shortcomings, such as in location procedures. For
known source regions, such as volcanoes, a well-oriented segment can leverage
continuous activity to record the incoming wavefield and extract dipersion curves
without the need to perform cross-correlations, simplifying the workflow.

How to cite: Latorre, H., Diaz-Meza, S., Jousset, P., Ventosa, S., Ugalde, A., Currenti, G., and Bartolomé, R.: Spectral analysis of background and transient signals at Mount Etna using rectilinear fibre-optic segments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5274, https://doi.org/10.5194/egusphere-egu26-5274, 2026.

EGU26-5880 | ECS | Posters on site | SM3.4

Enhancing High-frequency Ambient Noise for shallow subsurface imaging using urban ambient noise DAS recordings 

Leila Ehsaninezhad, Christopher Wollin, Verónica Rodríguez Tribaldos, and Charlotte Krawczyk

Distributed Acoustic Sensing (DAS) enables unused fiber optic cables in existing telecommunication networks, known as dark fibers, to function as dense arrays of virtual seismic receivers. Seismic waves generated by human activities and recorded by dense sensor networks provide an abundant, high-frequency energy source for high-resolution, non-invasive imaging of the urban subsurface. This approach enables detailed characterization of near-surface soils, sediments, and shallow geological structures with minimal surface impact, supporting applications such as groundwater management, site response and seismic amplification analysis, seismic hazard assessment, geothermal development, and urban planning. However, extracting coherent seismic signals from complex urban noise is challenging due to uneven source distribution, uncertain fiber deployment conditions, and variable coupling between the fiber and the ground. In particular, high-frequency range signals (e.g., above 4 Hz), needed to resolve shallow subsurface structures, are particularly difficult to recover. Two strategies can be used to address some of these challenges, by discarding poor quality seismic noise segments or by focusing on particularly favorable noise sources. In this study, we adopt the second approach and use vibrations generated by passing vehicles, particularly trains which are energetic sources that contain valuable high frequency information . Capturing and exploiting the seismic waves generated by these vehicles offers unique opportunities for efficient and high resolution urban seismic imaging.

We present an enhanced ambient noise interferometry workflow designed to exploit noise sources that are particularly favorable to the fiber geometry, i.e. transient and strong sources occurring at the edge of the fiber segment to be analyzed. The workflow is applied to traffic-dominated seismic noise recorded on a dark fiber deployed along a major urban road in Berlin, Germany. First, we select short seismic noise segments that contain signals from passing trains and then apply a frequency–wavenumber filter to isolate the targeted train-generated surface waves while suppressing other wavefield contributions. The filtered data is then processed using a standard interferometric approach based on cross-correlations to retrieve coherent seismic phases from ambient noise, producing virtual shot gathers. Finally, Multichannel Analysis of Surface Waves is applied to derive one dimensional velocity models. This workflow targeted on specific transient sources reduces computational cost while enhancing dispersion measurements particularly at higher frequencies. By stacking the responses from tens of tracked vehicles, enhanced virtual shot gathers can be obtained and inverted to improve shallow subsurface models. This can be achieved with only a few hours of seismic noise recording, which is challenging using conventional ambient noise interferometry workflows.

How to cite: Ehsaninezhad, L., Wollin, C., Rodríguez Tribaldos, V., and Krawczyk, C.: Enhancing High-frequency Ambient Noise for shallow subsurface imaging using urban ambient noise DAS recordings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5880, https://doi.org/10.5194/egusphere-egu26-5880, 2026.

EGU26-6600 | ECS | Posters on site | SM3.4

Multi-fiber Distributed Acoustic Sensing for Urban Seismology in Athens, Greece 

Mohammed Almarzoug, Daniel Bowden, Nikolaos Melis, Pascal Edme, Adonis Bogris, Krystyna Smolinski, Angela Rigaux, Isha Lohan, Christos Simos, Iraklis Simos, Stavros Deligiannidis, and Andreas Fichtner

Distributed Acoustic Sensing (DAS) offers a promising approach for dense seismic recording in urban environments by repurposing existing telecommunication infrastructure. Athens presents an ideal setting for such an approach, as Greece is one of the most seismically active countries in Europe, and the Athens metropolitan area — home to nearly four million inhabitants — lies within a geologically complex basin whose vulnerability was demonstrated by the destructive 1999 Mw 5.9 Parnitha earthquake. Seismic hazard assessment requires accurate subsurface velocity models, but acquiring the data to build them in dense urban areas remains challenging.

We present results from a multi-fiber DAS experiment conducted in Athens, Greece, from 16 May to 30 June 2025, using four telecommunication fibers provided by the Hellenic Telecommunications Organisation (OTE). Two Sintela ONYX interrogators simultaneously interrogated the four fibers, which fan out from an OTE building with lengths of approximately 24, 38, 42, and 48 km, providing extensive azimuthal coverage of Athens. This makes the study one of the largest urban DAS campaigns ever performed.

Data were acquired in two configurations, a lower spatial resolution mode optimised for earthquake recording (~26 days) and a higher resolution mode for ambient noise interferometry (~19 days). To detect seismic events, we applied bandpass filtering followed by phase-weighted stacking across channels to enhance coherent arrivals. An STA/LTA (short-time average/long-time average) trigger was then used to identify candidate events. During the acquisition period, the National Observatory of Athens (NOA) recorded 2,645 events across the broader seismic network, of which 548 were detected on at least one fiber (368, 343, 328, and 322 on fibers 1–4, respectively). Detection capability depends on distance and magnitude — we achieve near-complete detection within ~20 km, while many events of ML ≥ 2 were recorded at distances exceeding 200 km. The array also captured small local events absent from the NOA catalogue, likely corresponding to local seismicity below the detection threshold of the sparser regional network. Characterising this unobserved local seismicity is one of the objectives of ongoing work.

For events within 50 km of the interrogator site, we pick P- and S-wave arrivals to constrain body-wave travel times. These picks are used to locate events in the NOA catalogue, which enables us to compare with network-derived hypocentres and allows us to assess potential improvement from the dense DAS coverage, before applying the approach to smaller events detected only by DAS. The travel-time data will also serve as input for 3D eikonal traveltime tomography to image subsurface velocity structure beneath metropolitan Athens.

How to cite: Almarzoug, M., Bowden, D., Melis, N., Edme, P., Bogris, A., Smolinski, K., Rigaux, A., Lohan, I., Simos, C., Simos, I., Deligiannidis, S., and Fichtner, A.: Multi-fiber Distributed Acoustic Sensing for Urban Seismology in Athens, Greece, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6600, https://doi.org/10.5194/egusphere-egu26-6600, 2026.

EGU26-6949 | ECS | Posters on site | SM3.4

SAFE - Tsunami early warning system using available seafloor fiber cables with Chirped-pulse DAS 

Javier Preciado-Garbayo, Jaime A. Ramirez, Alejandro Godino-Moya, Jorge Canudo, Diego Gella, Jose Maria Garcia, Yuqing Xie, Jean Paul Ampuero, and Miguel Gonzalez-Herraez

Traditional tsunami early warning systems (TEWS) are typically expensive, have limited real-time availability, require continuous maintenance, and involve long deployment times. The SAFE project aims to overcome these limitations by developing a new tsunami warning technology based on Distributed Acoustic Sensing (DAS), leveraging existing seafloor fiber optic cables. This approach offers continuous 24/7 monitoring, near-zero maintenance, faster response times, and ease of installation. The project includes contributions ranging from the development of a novel Chirped-pulse DAS interrogator (HDAS) with improved low-frequency performance to a novel post-processing software to obtain tide height from the measured seafloor strain and automatic detection and confirmation of a tsunami wave. All this has been implemented in a friendly user interface and is undergoing final evaluation by the tsunami warning authority in the NE Atlantic (the Instituto Português do Mar e da Atmosfera, IPMA).  

The validation is currently ongoing using the ALME subsea cable, which connects Almería and Melilla across the Alboran Sea. The interrogator has demonstrated the ability to detect swell waves with a maximum error of 20 cm in the deep sea and a post-processing response time of less than 90 seconds. It is expected that slower tsunami waves will yield more precise estimations of wave height.

Importantly, the technology could also successfully detect the 5.3 Mw earthquake near Cabo de Gata, Spain, on July 14, 2025, at a distance of only 40 km from the epicenter without major saturation. The extremely large dynamic range of the interrogator (approximately 10 times larger than a usual phase system) enables the system to monitor large-magnitude earthquakes without signal clipping. The SAFE system is capable of delivering critical seismic and hydrodynamic data within 5 minutes of an event, supporting early tsunami detection and rapid response.

How to cite: Preciado-Garbayo, J., A. Ramirez, J., Godino-Moya, A., Canudo, J., Gella, D., Garcia, J. M., Xie, Y., Ampuero, J. P., and Gonzalez-Herraez, M.: SAFE - Tsunami early warning system using available seafloor fiber cables with Chirped-pulse DAS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6949, https://doi.org/10.5194/egusphere-egu26-6949, 2026.

EGU26-7247 * | ECS | Orals | SM3.4 | Highlight

Submarine Cable Optical Response to Seismic Waves: Insights from Controlled-Environment Tests 

Max Tamussino, David M. Fairweather, Ali Masoudi, Zitong Feng, Richard Barham, Neil Parkin, David Cornelius, Gilberto Brambilla, Andrew Curtis, and Giuseppe Marra

Fibre-optic sensing technology is transforming seafloor monitoring by enabling dense, continuous measurements across vast distances using existing telecommunication infrastructure. Distributed acoustic sensing (DAS) and optical interferometry [1] have demonstrated remarkable potential for earthquake detection, ocean dynamics monitoring, and hazard early warning. However, for these technologies to be used for these applications, the transfer function between environmental perturbations and measured optical signal changes in submarine cables needs to be known.

We present the, to the best of our knowledge, first controlled-environment characterisation of submarine cable responses to active seismic and acoustic sources, comparing DAS and optical interferometry measurements with ground-truth data from 58 geophones, 20 three-component seismometers, and microphones [2]. Our results reveal three key findings:

  • In contrast with proposed theoretical models [3], our interferometric measurements show first-order sensitivity to broadside seismic sources, enabling localisation of arrivals along straight fibre links.
  • We identify a previously unreported fast-wave phenomenon, attributed to seismic energy coupling into the cable's metal armour and propagating at velocities exceeding 3.5 km/s, significantly altering recorded waveforms.
  • We compared measurements between adjacent fibres within the same cable. Results show significant discrepancies between the measured waveforms, which should be considered in applications operating in a similar frequency range as our tests.

These findings show the complexity of submarine cable mechanics and their impact on optical sensing performance. Understanding these processes is critical for calibrating transfer functions and improving the reliability of fibre-based geophysical observations.  In addition to these findings, we also discuss the limitations of our methodology, which primarily arise from the limited range of seismic source frequencies available. Our work presents a first step towards understanding the complex transfer function of environmental perturbations to optical signals in subsea cables, advancing the vision of large-scale, cost-effective Earth observation systems.

[1] Marra, G. et al. Optical interferometry–based array of seafloor environmental sensors using a transoceanic submarine cable. Science 376 (6595), 874–879 (2022)

[2] Fairweather, D.M., Tamussino, M., Masoudi, A. et al. Characterisation of the optical response to seismic waves of submarine telecommunications cables with distributed and integrated fibre-optic sensing. Sci Rep 14, 31843 (2024)

[3] Fichtner, A., Bogris, A., Nikas, T. et al. Theory of phase transmission fibre-optic deformation sensing. Geophysical Journal International, 231(2), 1031–1039, (2022)

 

How to cite: Tamussino, M., Fairweather, D. M., Masoudi, A., Feng, Z., Barham, R., Parkin, N., Cornelius, D., Brambilla, G., Curtis, A., and Marra, G.: Submarine Cable Optical Response to Seismic Waves: Insights from Controlled-Environment Tests, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7247, https://doi.org/10.5194/egusphere-egu26-7247, 2026.

EGU26-7298 | ECS | Orals | SM3.4

Coastal Ambient Noise and Microseismic Monitoring with Distributed Acoustic Sensing: a Case Study from Norfolk, UK 

Harry Whitelam, Lidong Bie, Jessica Johnson, Andres Payo Garcia, and Jonathan Chambers

Seismic ambient noise is a ubiquitous and constant resource, ideal for non-invasive investigations of the solid earth. Coastlines around the world are handling an increase in coastal erosion due to sea level rise and more energetic storms. Monitoring this is becoming an increasingly necessary task to protect coastal settlements. Using Distributed Acoustic Sensing in seismic monitoring has already shown incredible potential and offers the advantage of dense measurements. Our project seeks to identify the efficacy of Distributed Acoustic Sensing for monitoring subsurface changes which precede cliff failure. We present early findings from the first long-term deployment of a fibre optic cable along the coastline - North Sea, Norfolk, UK. We investigate differences in signal characteristics between conventional seismometers and Distributed Acoustic Sensing in this setting, and interpret the seismic signatures of key sources in the area. This deployment was recording for 22 months, allowing us to monitor both short-term and seasonal changes. We identify the frequency ranges excited by storm events (0.2 - 1 Hz), the dominance of short-period secondary microseismic activity, and the importance of local sea state and weather on influencing higher frequency signals. We also discuss limitations of Distributed Acoustic Sensing and the sources it can not reliably capture when compared to broadband seismometers and nodal geophones. We conclude by discussing how this noise analysis affects the use of ambient noise tomography for seismic velocity monitoring. Future research will test the efficacy of such applications, with the hope of providing better estimates of coastal recession and identifying hazardous areas on a metre-scale.

How to cite: Whitelam, H., Bie, L., Johnson, J., Payo Garcia, A., and Chambers, J.: Coastal Ambient Noise and Microseismic Monitoring with Distributed Acoustic Sensing: a Case Study from Norfolk, UK, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7298, https://doi.org/10.5194/egusphere-egu26-7298, 2026.

EGU26-7427 | ECS | Orals | SM3.4

Distributed Fiber-Optic Sensing for Strain and Temperature Monitoring in an Underground Mine to Enable Digital Twin Integration 

Michael Dieter Martin, Nils Nöther, Erik Farys, Massimo Facchini, and Jens-André Paffenholz

The aim of this study is to assess the potential of distributed fiber-optic sensors for measuring strain and temperature in order to monitor the structural integrity of underground mining drifts and chambers. The work is conducted within the framework of the project “Model coupling in the context of a virtual underground laboratory and its development process” (MOVIE). The overall MOVIE project aim is intended to support the creation of a digital twin, thereby improving safety and operational efficiency through enhanced digital planning across various mining environments. Time-dependent, spatially distributed temperature and rock deformation data will be recorded along fiber-optic sensing cables. These measurements will serve as boundary conditions for integrated geometrical and geomechanical models of the drift and chambers. In the initial phase, a 60-meter-long drift is instrumented using fiber-optic Brillouin-based Distributed Temperature and Strain Sensing (DTSS). Based on laboratory tests and considering the specific environmental conditions of the subsurface mine, i.e., ambient temperature variations, surface roughness, dust, and humidity, the optimal adhesive bonding materials and technique for direct cable installation on gneiss host rock was identified and successfully implemented. Following the initial monitoring setup, further experimental investigations are planned, including the monitoring of induced deformations in yielding arch support, rock bolts and the rock in contact with a hydraulic prop. The drift geometry and the spatial location of the fiber-optic cables within the drift are given by a 3D point cloud. Therefore, a 3D point cloud was captured after the fiber-optic cable installation using a high-end mobile mapping SLAM platform geo-referenced in a project-based coordinate frame. The locations of the geo-referenced fiber-optic cables will be correlated with the acquired DTSS measurements along the fiber-optic sensing cables. Ultimately, the meshed 3D point cloud will serve as foundational input for the combined geometrical and geomechanical model, forming the basis for a virtual reality-compatible digital twin enriched with real-time sensor data.

How to cite: Martin, M. D., Nöther, N., Farys, E., Facchini, M., and Paffenholz, J.-A.: Distributed Fiber-Optic Sensing for Strain and Temperature Monitoring in an Underground Mine to Enable Digital Twin Integration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7427, https://doi.org/10.5194/egusphere-egu26-7427, 2026.

EGU26-7462 | Orals | SM3.4

Marine Distributed Acoustic Sensing (DAS) for Detection of Submarine CO₂ Bubble Emissions: Insights from a Shallow-Water Volcanic Setting at Panarea (Italy) 

Cinzia Bellezza, Fabio Meneghini, Andrea Travan, Luca Baradello, Michele Deponte, and Andrea Schleifer

Fibre-optic sensing technologies are rapidly transforming geophysical monitoring by enabling spatially dense, temporally continuous observations of seismic and acoustic wavefields in environments that are difficult to instrument with conventional sensors. In marine settings, Distributed Acoustic Sensing (DAS) applied to seabed fibre-optic cables offers new opportunities for low-impact monitoring of fluid and gas migration processes, which are fundamental both to volcanic–hydrothermal systems and to emerging offshore carbon capture and storage (CCS) applications.

In this study, we investigate the feasibility of marine DAS for detecting natural and artificial CO₂ bubble emissions in a shallow-water volcanic environment offshore Panarea (Aeolian Islands, Italy). Panarea hosts the OGS NatLab Italy, part of ECCSEL-ERIC, thanks to its active submarine degassing associated with a hydrothermal system and therefore represents a natural laboratory and an analogue site for potential subseabed CO₂ leakage scenarios. A 1.1-km-long armored fibre-optic cable was deployed on the seabed and interrogated using two different DAS systems, providing continuous passive acoustic and seismic recordings. To support signal identification and interpretation, the DAS data were complemented by controlled gas releases from scuba tanks, by a High Resolution Seismic (boomer) survey and side-scan sonar imaging, to characterize seabed morphology and shallow subsurface structures along the cable route.

The DAS recordings revealed acoustic signatures associated with both natural CO₂ bubble emissions and controlled artificial releases. Bubble-related signals were detected as localized, temporally variable acoustic responses along the fibre, demonstrating the sensitivity of DAS to gas-driven processes at the seabed. The integration of passive DAS monitoring with active seismic imaging techniques enabled a more robust interpretation of observed signals and seabed processes.

From an Earth sciences perspective, these results demonstrate that marine DAS can serve as a low-impact, spatially continuous monitoring tool for submarine volcanic and hydrothermal systems, complementing traditional geochemical sampling and visual observations and offering new insights into the temporal variability of degassing activity. Beyond natural systems, the demonstrated capability of DAS to detect bubble-related acoustic signals has direct implications for offshore CCS, where early detection of CO₂ leakage is critical for storage integrity and environmental safety.

Overall, this field-scale experiment highlights the potential of fibre-optic sensing to address key challenges in marine monitoring, and underscores the value of integrated approaches for studying fluid and gas migration processes.

Acknowledgements:

  • ECCSELLENT project (“Development of ECCSEL - R.I. ItaLian facilities: usEr access, services and loNg-Term sustainability”)
  • ITINERIS - Italian Integrated Environmental Research Infrastructures System - Next Generation EU Mission 4, Component 2 - CUP B53C22002150006 - Project IR0000032
  • Panarea NatLab Italy: https://eccsel.eu/catalogue/facility/?id=124
  • ECCSEL: https://eccsel.eu/

 

References:

  • Detection of CO2 emissions from Panarea seabed with Distributed Acoustic Sensing (DAS): a preliminary investigation. Meneghini et al. OGS report (2025).
  • Marine Fiber-Optic Distributed Acoustic Sensing (DAS) for Monitoring Natural CO₂ Emissions: A Case Study from Panarea (Aeolian Islands, Italy). Bellezza et al. Upon submission to Applied Sciences (2026).

How to cite: Bellezza, C., Meneghini, F., Travan, A., Baradello, L., Deponte, M., and Schleifer, A.: Marine Distributed Acoustic Sensing (DAS) for Detection of Submarine CO₂ Bubble Emissions: Insights from a Shallow-Water Volcanic Setting at Panarea (Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7462, https://doi.org/10.5194/egusphere-egu26-7462, 2026.

EGU26-7987 | ECS | Orals | SM3.4

Urban-Scale Seismic Imaging Using Ambient Noise and Dark Fiber Distributed Acoustic Sensing in Istanbul 

Laura Pinzon-Rincon, Verónica Rodríguez Tribaldos, Jordi Jordi Gómez Jodar, Patricia Martínez-Garzón, Laura Hillmann, Recai Feyiz Kartal, Tuğbay Kılıç, Marco Bohnhoff, and Charlotte Krawczyk

Urban areas are highly vulnerable to the impacts of geohazards due to their dense populations and complex infrastructure, with potentially severe consequences for human life and economic stability. Improving our knowledge of near-surface and shallow subsurface structures in urban environments is therefore essential for effective seismic hazard assessment and risk mitigation. However, conventional geophysical surveys in cities are often limited by logistical constraints, including strong anthropogenic activity, restricted access, legal limitations, and risks associated with instrument deployment. In this context, repurposing existing telecommunication optical fibers (so-called dark fibers) as dense seismic sensing arrays using Distributed Acoustic Sensing (DAS) offers a powerful alternative for urban subsurface investigations. This approach enables continuous, high-resolution seismic monitoring without the need for extensive field instrumentation.

The megacity of Istanbul (Turkey) is located in one of the most tectonically active regions worldwide and is exposed to significant seismic hazard. Since May 2024, we have been continuously recording passive seismic data using Distributed Acoustic Sensing (DAS) along an amphibious fiber-optic cable, is deployed in the urban district of Kartal (eastern region of Istanbul) and immediately offshore. In this study, we focus on the 3 km-long urban segments of the fiber. We analyze ambient seismic noise generated by various anthropogenic sources, such as train and vehicle traffic and other urban activities, and evaluate their suitability for high-frequency, DAS-based passive seismic interferometry in a complex and heterogeneous urban setting.

We develop and adapt processing strategies for ambient-noise interferometry that address the challenges of dense urban environments and DAS array geometries, including the identification of suitable fiber sections, channels, and source-receiver configurations, as well as preprocessing schemes designed for strongly anthropogenic noise.The objective is to retrieve high-resolution, urban-scale subsurface velocity models that improve our understanding of shallow structures and material properties relevant to seismic hazard. Ultimately, this work aims to establish efficient methodologies for imaging the urban subsurface using existing infrastructure, contributing to improved geohazard assessment and supporting sustainable urban development in seismically active regions.

How to cite: Pinzon-Rincon, L., Rodríguez Tribaldos, V., Jordi Gómez Jodar, J., Martínez-Garzón, P., Hillmann, L., Feyiz Kartal, R., Kılıç, T., Bohnhoff, M., and Krawczyk, C.: Urban-Scale Seismic Imaging Using Ambient Noise and Dark Fiber Distributed Acoustic Sensing in Istanbul, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7987, https://doi.org/10.5194/egusphere-egu26-7987, 2026.

Applied to existing but underutilized fiber-optic networks (dark fibers), Distributed Acoustic Sensing (DAS) offers an attractive approach for large-scale seismic monitoring with minimal deployment effort. However, the approach introduces specific challenges, as existing infrastructures were not designed for this purpose, leading to constraints related to sensor coupling, heterogeneous installation conditions, and limited characterization of the measurement points. In the frame of the RUBADO project, we investigate the potential and limitations of DAS applied to dark fibers to provide seismic observations supporting both operational monitoring and characterization of deep geothermal reservoirs. The approach is implemented at multiple spatial scales within the Upper Rhine Graben, where several geothermal plants are currently operating, under development, or in the planning phase. In this context, research activities within the project specifically target key practical challenges related to the use of DAS on dark-fibers for the seismic monitoring of geothermal reservoirs.

Currently, data are recorded along a ~20 km fiber-optic line using the KIT infrastructure, which will support the monitoring of the drilling of a 1.4 km-deep geothermal well at KIT Campus North. We present early results from local and regional seismic monitoring and associated methodological approaches for signal enhancement and seismic event detection. We also introduce a framework for subsurface characterization that leverages the frequent vehicle-generated signals observed in the DAS recordings. We then outline planned measurements at the scale of the Upper Rhine Graben, where a key feature is the simultaneous use of multiple dark-fiber lines. Given the geometry of the planned dark-fiber network, DAS observations will enable the simultaneous monitoring of several geothermal sites with favorable spatial coverage.

How to cite: Azzola, J. and Gaucher, E.: Seismic monitoring of geothermal reservoirs using Distributed Acoustic Sensing on dark fibers: the RUBADO project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8212, https://doi.org/10.5194/egusphere-egu26-8212, 2026.

EGU26-8268 | ECS | Posters on site | SM3.4

Seismic monitoring of alpine lake ice with distributed acoustic sensing (DAS) and nodal arrays 

Ariana David, Cédric Schmelzbach, Thomas Hudson, John Clinton, Elisabetta Nanni, Pascal Edme, and Frederik Massin

Lake ice stability is critical for safe operations on mid- to high-altitude Alpine lakes, such as touristic activities. Existing lake-ice monitoring approaches like ground-penetrating radar and drilling are limited in their ability to resolve spatial variability and to enable continuous monitoring and require direct access to the ice for in situ measurements. Seismological methods offer a complementary approach by recording the wave field generated by lake-ice flexure and fracturing. Here, we assess Distributed Acoustic Sensing (DAS) as a long-term seismic monitoring tool for Alpine lakes.

During Winter 2025, we deployed two complementary seismic sensing systems on frozen Lake Sankt Moritz in the Swiss Alps: a fibre-optic network for DAS measurements and an array of over 40 three-component conventional autonomous seismic nodes to benchmark performance. We installed more than 2 km of fibre-optic cable and connected two interrogators that recorded, over a few weeks, strain and strain-rate data in two cores within the same cable.

To characterise ice properties and icequakes, we implemented workflows for automated icequake detection and location using the waveform-coherency based QuakeMigrate framework, which does not require phase picking, alongside an approach based on semi-automatic phase identification and picking. We successfully detected and located events with both types of instrument networks. Using a baseline catalogue from the three-component node data, we evaluated the DAS performance and achieved location agreement within a few metres between different sensing systems, demonstrating that DAS can robustly capture and localise icequake activity on lake ice and is a promising tool for continuous ice-stability monitoring.

How to cite: David, A., Schmelzbach, C., Hudson, T., Clinton, J., Nanni, E., Edme, P., and Massin, F.: Seismic monitoring of alpine lake ice with distributed acoustic sensing (DAS) and nodal arrays, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8268, https://doi.org/10.5194/egusphere-egu26-8268, 2026.

EGU26-8383 | ECS | Orals | SM3.4

Distributed acoustic sensing of very long period strain signals from strombolian explosions 

Francesco Biagioli, Eléonore Stutzmann, Pascal Bernard, Jean-Philippe Métaxian, Valérie Cayol, Giorgio Lacanna, Dario Delle Donne, Yann Capdeville, and Maurizio Ripepe

Very long period (VLP; 0.01-0.2 Hz) seismicity is observed at many volcanoes worldwide, and provides key insights into magma and fluid dynamics within volcanic structures. VLPs are typically recorded by sparse networks of seismometers, which limits the ability to resolve the resulting displacement (or deformation) at fine spatial scales. Distributed acoustic sensing (DAS) may help overcome this limitation by densely sampling the projection of the strain tensor along fibre-optic cables with high spatial and temporal resolution, enabling a more complete view of VLP-induced deformation. Here, we analyse VLP strain signals recorded by DAS at Stromboli volcano (Italy) in November 2022 along a 6-km dedicated fibre-optic cable. We designed the cable geometry to provide broad coverage of the craters and to sample the strain at multiple locations and along different directions. We focus on a dataset of approximately 200 VLP events recorded between November 13 and 14, 2022. The VLP strain signals correlate with explosive activity and show consistent features across multiple events, indicating a persistent, non-destructive source. Leveraging the distributed nature of DAS measurements, we recover the principal strain axes of VLPs and estimate both the location and the volumetric change of the source using a quasi-static deformation model. We retrieve the principal horizontal strains for each VLP by inverting strain amplitudes measured along three different fibre directions and at multiple locations along the cable, allowing us to resolve their spatial distribution. The resulting principal VLP strains exhibit radial and tangential orientations with respect to the craters, consistent with observed seismic particle motions and an axisymmetric source. We then model the VLP strain along the fibre using a point-like deformation source (Mogi). The optimal agreement between modeled and observed VLP strain averaged over the 200 events is for a point source located ~500 m beneath the active craters, with an estimated volumetric change of ~30 m³. Under the assumption of a spherical source with a radius of 87 m, the inferred volumetric change corresponds to a pressure change of ~19 kPa. These results are consistent with previous studies and highlight the capability of DAS to investigate volcano deformation at long periods.

How to cite: Biagioli, F., Stutzmann, E., Bernard, P., Métaxian, J.-P., Cayol, V., Lacanna, G., Delle Donne, D., Capdeville, Y., and Ripepe, M.: Distributed acoustic sensing of very long period strain signals from strombolian explosions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8383, https://doi.org/10.5194/egusphere-egu26-8383, 2026.

EGU26-8769 | ECS | Posters on site | SM3.4

Analyzing volcanic-like earthquakes with distributed acoustic sensing using a short segment of the Tongan seafloor telecommunications cable 

Shunsuke Nakao, Mie Ichihara, Masaru Nakano, Taaniela Kula, Rennie Vaiomounga, and Masanao Shinohara

The January 2022 eruption of the Hunga Tonga-Hunga Ha'apai (HTHH) volcano highlighted the critical challenges in monitoring remote submarine volcanic activity. Distributed Acoustic Sensing (DAS) utilizing existing seafloor telecommunications cables offers a promising solution to bridge this observational gap. We analyzed a one-week DAS dataset recorded in February 2023, approximately one year after the eruption, using a segment of a domestic telecommunication cable in Tonga.

While a previous analysis of this dataset focused on relatively large events with clear phases, our objective was to comprehensively detect small and unclear seismic signals to evaluate the post-eruption activity. We developed a new "duration-based" detection method that identifies temporally sustained energy increases in the array's median power, effectively suppressing spatially incoherent noise. This method successfully detected 770 discrete events, revealing a stable seismicity rate of approximately 110 events per day, significantly more than those detected by conventional triggering algorithms.

To distinguish the origin of these events, we estimated the apparent slowness of the signals using a robust method combining 2D Normalized Cross-Correlation and linear fitting (RANSAC). The results showed that most events have positive apparent slowness values, corresponding to arrivals from the direction of the HTHH volcano, rather than the negative apparent slowness corresponding to tectonic earthquakes from the Tongan Trench. These findings indicate that the HTHH volcano or its surrounding magmatic system maintained a high level of seismic activity even one year after the large 2022 eruption. This study demonstrates the capability of DAS to monitor subtle volcanic seismicity in submarine environments where traditional sensors are absent.

How to cite: Nakao, S., Ichihara, M., Nakano, M., Kula, T., Vaiomounga, R., and Shinohara, M.: Analyzing volcanic-like earthquakes with distributed acoustic sensing using a short segment of the Tongan seafloor telecommunications cable, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8769, https://doi.org/10.5194/egusphere-egu26-8769, 2026.

EGU26-9174 | ECS | Posters on site | SM3.4

Clustering of Large Distributed Acoustic Sensing Datasets 

Oliver Bölt, Conny Hammer, and Céline Hadziioannou

Distributed Acoustic Sensing (DAS) turns optical fibers into high resolution strain sensors by monitoring the scattering of light within the fiber. With channel distances in the order of a few meters and a typical sampling frequency of 1 kHz, DAS is capable of recording a wide range of natural and anthropogenic seismic signals. Furthermore, the optical fibers used for DAS can be several kilometers long and are suitable for long-term measurements over weeks, months or years. The datasets obtained by DAS can therefore be very large, with up to several terabytes of data per day. Due to this large amount of data, it is challenging to get a good overview of the different types of seismic signals contained in the data, since a manual inspection can become immensely time-consuming.

In this study we aim to automatize this process by clustering the data to detect and classify different types of seismic signals.  A two-dimensional windowed Fourier transform is used to automatically extract features from the data. In contrast to many other approaches, this allows to not only use temporal information, but to also include the spatial dimension to further distinguish between different seismic sources and wave types.

The clustering is performed in two steps. First, a Gaussian Mixture Model (GMM) is used to cluster the feature set. Then, the final clusters are obtained by merging similar components of the GMM.

A key advantage of this method is that each final cluster represents a specific frequency distribution and can therefore be turned into a filter. While many clustering approaches only assign a list of labels or cluster memberships to the data, our method provides the ability to directly extract the characteristic seismic signals for each cluster. This helps greatly with cluster interpretation and can also be useful for further applications like event detection or denoising.

The proposed procedure is applied to different large DAS datasets, yielding a variety of different clusters. By filtering the data for each cluster and interpreting the obtained waveforms, as well as the long-term spatiotemporal amplitude patterns, different sources like traffic or machinery can be identified.

How to cite: Bölt, O., Hammer, C., and Hadziioannou, C.: Clustering of Large Distributed Acoustic Sensing Datasets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9174, https://doi.org/10.5194/egusphere-egu26-9174, 2026.

EGU26-10581 | ECS | Posters on site | SM3.4

Urban Seismology of a Popular Road Race Using Distributed Acoustic Sensing 

Jorge Canudo, Diego Gella, Pascual Sevillano, and Javier Preciado-Garbayo

Distributed Acoustic Sensing (DAS) has emerged as a powerful tool for monitoring human-induced seismic signals in urban environments, enabling dense, meter-scale observations of dynamic sources. Building on previous studies demonstrating the capability of DAS to image large public events, such as parades and other mass-participation activities, we present a novel experiment in which two different DAS technologies (ΦOTDR and Chirped-Pulse ΦOTDR) were simultaneously deployed to record a popular pedestrian road race held in the surroundings of the University of Zaragoza (Spain).

The experiment took advantage of an already deployed optical-fiber installation with a total effective length of approximately 2 km. The fiber layout captured three distinct geometrical configurations with respect to the race course: (1) a straight section coincident with the runners’ trajectory over the last 300 m of the first kilometer (outbound leg), (2) the same straight section during the return at kilometer 4 (inbound leg), and (3) a perpendicular crossing of the fiber with the race course at the finish line. This geometry provides a unique opportunity to analyze runner-induced ground vibrations under varying crowd densities, running speeds, and fiber–source orientations.

Waterfall representations of the strain-rate data reveal clear, coherent signatures associated with individual runners and runner groups in both DAS systems. Along the straight section, the outbound leg exhibits a compact, high-amplitude wavefield characterized by closely spaced, overlapping runner traces, consistent with the tightly packed peloton early in the race. In contrast, the inbound leg shows a markedly more dispersed pattern, reflecting the progressive spreading of participants according to performance and fatigue. These differences are consistently observed in both phase-based and chirped-pulse DAS data, although with distinct signal-to-noise characteristics across different frequency bands.

At the finish line, where the fiber crosses the race course perpendicularly, the DAS records provide exceptional temporal resolution of runner arrivals. The first five finishers are individually and unambiguously identified, with isolated signatures that can be robustly matched to official arrival times. This demonstrates the potential of DAS not only for bulk crowd characterization but also for resolving individual human-induced seismic sources in real-world conditions.

Our results highlight the complementarity of DAS technologies for urban seismology applications. The experiment underscores the sensitivity of DAS to subtle variations in crowd dynamics and source geometry and illustrates its potential for non-intrusive monitoring of mass-participation events, pedestrian flows, and urban activity. These observations contribute to the growing field of anthropogenic seismology and reinforce the role of optical fiber sensing as a scalable tool for high-resolution monitoring of human activity in cities.

How to cite: Canudo, J., Gella, D., Sevillano, P., and Preciado-Garbayo, J.: Urban Seismology of a Popular Road Race Using Distributed Acoustic Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10581, https://doi.org/10.5194/egusphere-egu26-10581, 2026.

EGU26-10676 | Orals | SM3.4

Storm Amy observations with fibre-optic DAS data at the Svelvik CO₂ Field Lab, Norway: Implications for Monitoring and Networks  

Claudia Pavez Orrego, Marcin Duda, Dias Urozayev, Bastien Dupuy, and Nicolas Barbosa

Distributed Acoustic Sensing (DAS) has become a powerful technique for high-resolution, continuous monitoring of near- and subsurface earth phenomena, with increasing applications in geohazards, seismology, and industry applications such as CO₂ storage monitoring. However, the sensitivity of DAS measurements to atmospheric forcing, particularly during extreme weather events, remains poorly understood. In this study, we investigate the response of a permanent, 1.2 km long straight fibre-optic array installed at the Svelvik CO₂ Field Laboratory (Norway), to intense wind conditions associated with the Amy Storm, which hit Norway from October 3-6, 2025. 

 

As part of efforts to understand passive methods to monitor CO2 migration in the subsurface, an Alcatel Submarine Networks (ASN) DAS system continuously recorded strain-rate data along a buried fibre that includes both near surface-installed sections and borehole down- and up-going segments reaching depths of approximately 100 m. The near-surface sections were installed inside protective pipes and were therefore not directly coupled to the surrounding ground. To characterise wind-induced seismic signatures, we analyse downsampled recordings using band-limited root-mean-square (RMS) amplitudes and spectral methods across three frequency ranges (0.1–1 Hz, 1–3 Hz, and 3–10 Hz) and time averages over 1 hr intervals. Time–frequency characteristics are examined using group-averaged spectrograms, and a Spectral Energy Index (SEI) is derived by integrating power spectral density within each frequency band. These seismic metrics are compared with near located meteorological observations, including mean wind speed, maximum mean wind speed, and maximum wind gusts. 

 

The results reveal a pronounced increase in DAS energy coincident with the maximum speed gusts of storm Amy, with the strongest responses observed at frequencies below 3 Hz. Correlation and lag analyses show that seismic energy variations are closely associated with periods of enhanced wind activity, particularly wind gusts, indicating a strong coupling between transient atmospheric forcing and ground vibrations. Importantly, the response differs significantly between surface and depth segments of the fibre. Surface-installed channels exhibit broadband amplitude increases correlated with direct wind–ground interaction, while depth channels display coherent low-frequency spectral patterns, suggesting excitation by wind-generated surface waves or distant secondary sources (e.g., waves from neighbouring fjord) rather than direct aerodynamic loading. 

 

These findings demonstrate that DAS arrays deployed at wells (abandoned or active) are sensitive to extreme meteorological forcing, which can imprint distinct and depth-dependent seismic signatures. Quantifying and distinguishing wind-induced signals is therefore critical for the robust interpretation of DAS data in long-term passive monitoring applications, particularly when subtle subsurface signals related to CO₂ injection, migration, or leakage must be detected in the presence of strong environmental noise. At the same time, this sensitivity highlights an additional benefit of such fibre-optic installations: DAS infrastructure deployed in future abandoned wells in the context of  Oil & Gas industry and their reutilization for CO2 capture and storage, can also provide valuable information for national seismic and environmental monitoring networks, extending their utility beyond site-specific applications. 

How to cite: Pavez Orrego, C., Duda, M., Urozayev, D., Dupuy, B., and Barbosa, N.: Storm Amy observations with fibre-optic DAS data at the Svelvik CO₂ Field Lab, Norway: Implications for Monitoring and Networks , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10676, https://doi.org/10.5194/egusphere-egu26-10676, 2026.

EGU26-10839 | ECS | Posters on site | SM3.4

Fibre sensing at regional scales with telecom cables: the IMAGFib project 

Nicolas Luca Celli, Chris Bean, Adonis Bogris, Georgios Aias Karydis, Eoin Kenny, Rosa Vergara, Örn Jónsson, and Marco Ruffini

Fibre sensing technology can provide seismic data at a variety of scales, but, currently, the difficulty in accessing long telecom fibres, together with the novelty of the instruments, their range limitations and massive data output, mostly constrain its applications to fibre <100 km long.

In this study, we showcase the first results from the new project IMAGFib (multiscale seismic IMAGing with optical FlBre telecom cables), acquiring on-/offshore fibre sensing data on commercial telecom fibres in the North Atlantic Ocean, Irish Sea and across Ireland. This project combines utilising Distributed Strain Sensing (DSS, also known as DAS) on >400 km with 10 m spatial sampling with a new, distributed Microwave Frequency Fiber Interferometer (MFFI) capable sensing over 1700 km of submarine cables connecting Ireland to Iceland, albeit with a coarser 50-100 km spatial sampling. We use the acquired data to assess the performance of fibre sensing as a regional-to-continental scale seismic and ocean monitoring, and a future imaging tool, with a focus on low frequencies (<1 Hz).

By forging research collaborations with multiple telecom operators, we are able to perform DSS on multiple cable sections across the region, aiming to cover a continuous linear profile from Wales to the North Atlantic through different experiments (to be completed early 2026), part of which is performed on live, traffic-carrying telecom fibres. Our DSS results show that while having lower signal to noise ratios compared to nearby seismic stations, DSS on noisy telecom fibres can successfully record most Mw>6 teleseismic events worldwide, as well as microseisms originating in the North Atlantic and/or Irish Sea on all sections of the cable.

In order to extend fibre sensing far into the North Atlantic Ocean, we present the newly developed MFFI sensor, which uses optical interferometry in conjunction with high-loss loop backs at line amplifiers, turning each section of the cable between amplifiers (50-100 km) into independent strain sensors. For our experiment on the Ireland-Iceland cable, this yields 17 traces along the fibre. Ongoing recording in late 2025-early 2026 allows us to evaluate its capability to sense seismic signals, marine storms, currents and possibly ocean-bottom temperature variations across seasons.

With a strong focus on long-range and low-frequency sensing and integration with live telecom infrastructure, IMAGFib is centred on the establishment of fibre sensing as a global geo-sensing tool. Our successful results using DSS on live telecom fibres, and developing MFFI technology using affordable off-the-shelf components represent a key step in advancing the efforts to broaden trusted research utilising existing, commercial telecom cables.

How to cite: Celli, N. L., Bean, C., Bogris, A., Karydis, G. A., Kenny, E., Vergara, R., Jónsson, Ö., and Ruffini, M.: Fibre sensing at regional scales with telecom cables: the IMAGFib project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10839, https://doi.org/10.5194/egusphere-egu26-10839, 2026.

EGU26-11265 | ECS | Posters on site | SM3.4

SmartScape: Distributed Strain Sensing on Dublin City Telecom Fibre to Monitor Urban and Subsurface Dynamics for Smart City Applications 

Bruna Chagas de Melo, Christopher J. Bean, and Colm Browning

Rapid urban growth in Dublin is placing increasing pressure on transport systems, construction activity, and environmental management, creating a clear need for high-resolution observations of how the city operates at both surface and subsurface levels. This study presents the initial stage of a new project that explores the feasibility of using existing optical telecommunication infrastructure as a large-scale urban sensing platform through Distributed Strain Sensing (DSS). DSS converts optical fibres into dense seismic arrays by measuring strain-rate perturbations caused by ground vibrations, offering a cost-efficient approach to city-scale monitoring. This can have a potentially transformative impact on smart and sustainable city management, offering new data insights into urban dynamics while leveraging existing city-owned fibre infrastructure.

We report on a first pilot deployment on a dark ~80 km fibre ring crossing the city centre, residential neighbourhoods, surface tram lines, and an underground tunnel. A FEBUS-A1 interrogator was installed at a data centre in Dublin’s north side and operated for 23 days. Several acquisition configurations were tested, with the most stable setup recording ~60 km of fibre at 500 Hz sampling and 20 m gauge length for a continuous 10-day period. Remote access enabled iterative optimisation of acquisition parameters during the experiment.

The analysis presented here is preliminary and focuses on assessing data quality, signal content, and key technical limitations. Initial observations indicate that the DSS array captures clear signatures of moving vehicles with different velocities, rail-related activity, and teleseismic signals, including the October 10th M7.4 Mindanao, Philippines event. Signal quality progressively degrades beyond ~30 km from the interrogator, where noise becomes dominant, highlighting challenges associated with attenuation, coupling, and urban noise in long fibre links.

Ongoing work focuses on developing denoising and source-identification strategies, including cross-correlation approaches and unsupervised machine-learning, alongside accurate georeferencing of fibre channels onto detailed urban maps. These analyses will be integrated with independent datasets such as traffic records from Dublin City Council and existing environmental acoustic noise maps. Rather than delivering operational products, this study is intended to establish a robust baseline on data quality, signal content, and interpretability, defining what information can realistically be extracted from urban DSS deployments in Dublin at this early stage.

How to cite: Chagas de Melo, B., J. Bean, C., and Browning, C.: SmartScape: Distributed Strain Sensing on Dublin City Telecom Fibre to Monitor Urban and Subsurface Dynamics for Smart City Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11265, https://doi.org/10.5194/egusphere-egu26-11265, 2026.

EGU26-11391 | Posters on site | SM3.4

Integrating Distributed Acoustic Sensing and borehole seismometer data for seismic velocity measurements and negative magnitude event location: a case study from the TABOO Near Fault Observatory (Northern Apennines, Italy) 

Nicola Piana Agostinetti, Federica Riva, Irene Molinari, Simone Salimbeni, Alberto Villa, Marta Arcangeli, Giulio Poggiali, Raffaello Pegna, Gilberto Saccorotti, Gaetano Festa, and Lauro Chiaraluce

Distributed Acoustic Sensing (DAS) technology makes use of fiber optic cables to sense vibrations, at the Earth’s surface, at unprecedented spatial resolution, less than one meter over distances of kilometres. DAS data have been used for monitoring both the Solid Earth (earthquakes, dyke intrusions and more) and the environment (landslides, snow avalanches, groundwater). Despite its wide application and the numerous, successful case-studies, DAS technology presents two significant limitations: the lower S/N ratio with respect to standard seismometers and the strong "directivity effect" (vibrations must propagate in the axial direction of the fiber optic cable). In this study, we illustrate how the integration of DAS and borehole seismometer data can be used to improve earthquake location and obtain novel information on seismic velocity of the buried rock mass. We analyse the DAS data recorded along a 1km fiber optic cable deployed in a full 3D geometry. The fiber optic cables have been installed in the framework of a surface and borehole very dense seismic array partaining to the Alto Tiberina Near Fault Observatory (TABOO-NFO). The cable geometry covers two horizontal planes, off-set one from the other and at different altitudes, and a vertical borehole  going to 130m depth. The infrastructure has been installed across (from the hangingwal to the footwall) the Gubbio fault, a secondary fault segment antithetic to the main Alto Tiberina master fault bounding at depth a normal fault system. in the Alto Tiberina fault system (Northern Apennines, Italy). The center of the cable array coincides with a shallow borehole (130m deep)  instrumented with two short period seismometers, one at the surface and one at the bottom. The integration of the data from the seismometes and those recorded along such 3D geometry allows for a better recognition and location of very small seismic events occurring on the fault, which are going largely undetected by the local (dense) seismic network. Moreover, data from small size events (Mag > 1) can be used to estimate the P- and S- wave seismic velocity of the geological formation traversed by the borehole (namely, Maiolica fm and Marne a Fucoidi fm), defining precise measurements of such velocities at larger scale-length (10s of meters) with respect to measurements obtained on the same rock in the laboratory.

How to cite: Piana Agostinetti, N., Riva, F., Molinari, I., Salimbeni, S., Villa, A., Arcangeli, M., Poggiali, G., Pegna, R., Saccorotti, G., Festa, G., and Chiaraluce, L.: Integrating Distributed Acoustic Sensing and borehole seismometer data for seismic velocity measurements and negative magnitude event location: a case study from the TABOO Near Fault Observatory (Northern Apennines, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11391, https://doi.org/10.5194/egusphere-egu26-11391, 2026.

EGU26-11798 | ECS | Posters on site | SM3.4

Distributed Acoustic Sensing of debris-flow activity in the Öschibach torrent (Swiss Alps) 

Juan Sebastian Osorno Bolivar, Malgorzata Chmiel, Fabian Walter, Felix Blumenschein, and Kevin Friedli

The slope instability of Spitze Stei supplies large sediment volumes that accumulate at the slope toe and are subsequently remobilized as debris flows and debris floods in the adjacent Öschibach torrent thus threatening the nearby village of Kandersteg, Switzerland. Since early 2020, continuous monitoring and preventive measures have been implemented in the area. While long-term monitoring has documented frequent torrential activity, the dynamic linkage between sediment supply from the rock slope and debris-flow activity in the torrent remains poorly constrained due to the spatial limitations of point sensors.

In summer 2025, we deployed a dense seismic array on the rock slope and interrogated an existing dark optical fiber running along the ~4 km-long Öschibach torrent using Distributed Acoustic Sensing (DAS). The DAS setup enabled spatially continuous strain-rate measurements at meter-scale resolution with a sampling frequency of ~600 Hz. For the three-month acquisition period, our aim is to detect and characterize debris-flow and debris-flood activity using DAS methods, supported by relative water-level time series and data from nearby seismic stations.

A catalog of possible debris flows and debris floods is generated leveraging an established pre-warning water-level increase threshold (set at 0.6 m), using moving average windowing and duration filtering. This discharge inventory was characterized using the DAS array, whose ~850 channels have been geolocalized with tap test, based on strain rate amplitudes visualized in logarithmic waterfall plots. Analysis of Power Spectral Density (PSD) for the corresponding DAS recordings reveals an increase in seismic energy at high frequencies (~20-40 Hz) concentrated on channels closest to the stream. Vertically offset waveform comparison plots demonstrate high coherence between DAS channels and wavefields recorded at the seismic stations, from which the apparent speed of seismic sources can be estimated. We also observe other coherent signals along the fiber, including mass movements from the Spitze Stei rock slope (e.g., rockfalls and granular flows), as well as local and tele-seismic earthquakes.

Our assessment of signal quality and coherence provides a basis for subsequent event detection, source location, and characterization using array-based methods, particularly during the event initiation phase. Our multisensor approach highlights the potential of DAS to provide spatially dense observations of torrential processes in steep Alpine catchments.

How to cite: Osorno Bolivar, J. S., Chmiel, M., Walter, F., Blumenschein, F., and Friedli, K.: Distributed Acoustic Sensing of debris-flow activity in the Öschibach torrent (Swiss Alps), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11798, https://doi.org/10.5194/egusphere-egu26-11798, 2026.

EGU26-12160 | ECS | Orals | SM3.4

Best Practices for Machine Learning based Icequake Picking with Distributed Acoustic Sensing 

Johanna Zitt, Marius Isken, Jannes Münchmeyer, Dominik Gräff, Andreas Fichtner, Fabian Walter, and Josefine Umlauft

Over the past years, a wide range of machine learning–based phase picking methods have been developed, primarily targeting three-component seismometer data from tectonic earthquakes. With the rapid growth of distributed acoustic sensing (DAS) applications, diversification of use cases, and availability of increasingly large DAS datasets, these methods are now being applied to single-component DAS recordings. However, their optimal use for DAS data and for alternative signal types such as cryoseismological events, remains rarely explored.
In this study, we present a systematic analysis of the performance of machine learning–based phase picking methods pretrained on tectonic earthquakes on one-component cryoseismological DAS data obtained on the Rhône Glacier in the Swiss Alps in July 2020. We evaluate multiple strategies for generating pseudo-three-component data from the intrinsically single-component DAS strain-rate data, including zero-padding of missing components, duplication of the single component, and the use of consecutive DAS channels as surrogate components. In addition, we assess the phase-picking performance across different preprocessing schemes, comparing conservatively band-pass filtered data with denoised data obtained using a J-invariant  autoencoder specifically trained on cryoseismological DAS data. Finally, we analyze the spatial and temporal distribution of located events over the full observation period and across the entire glacier. Event clusters are correlated with weather conditions, daily cycles, and the geometry of the glacier bed to explore potential patterns in cryoseismic activity.
Our results indicate that treating consecutive DAS channels as surrogate components yields the most reliable phase-picking performance, whereas extensive denoising can degrade picking accuracy. We further discuss spatial clusters of event locations and their correlations with glacier topography and meteorological conditions.

How to cite: Zitt, J., Isken, M., Münchmeyer, J., Gräff, D., Fichtner, A., Walter, F., and Umlauft, J.: Best Practices for Machine Learning based Icequake Picking with Distributed Acoustic Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12160, https://doi.org/10.5194/egusphere-egu26-12160, 2026.

EGU26-12365 | ECS | Posters on site | SM3.4

Distributed Acoustic Sensing (DAS) for Geothermal Applications: a Case Study Across Dublin City 

Eoghan Totten, Jean Baptiste Tary, and Bruna Chagas de Melo

Seismic monitoring plays an integral role in geothermal renewable energy projects for imaging, site-specific noise characterisation and hazard risk assessment purposes. The number of European geothermal energy projects is expected to rise over the next decade as efforts to mitigate for reliance on fossil fuel-derived energy sources continue. Related to this is the pressing need to prospect for and expand the use of geothermal energy in urban settings.

Distributed Acoustic Sensing (DAS) is increasingly applied in lieu of geophone-based deployments. Instead of measuring seismic waves at a limited number of discrete points, DAS transforms fibre-optic cables into large and dense arrays of virtual sensors by measuring small changes in strain rate, with gauge length resolutions as small as 1-20 metres. DAS interferometry is able to capitalise on extant urban fibre-optic infrastructure, as well as exploit the diverse and passive seismic noise sources available in towns and cities.

Here we present in-progress DAS data analysis from an approximately 70-80km long cable crossing Dublin city (south to north) for three weeks of cumulative recording between September-October 2025. This cable tracks a large portion of the M50 ring road, the main arterial traffic route between north and south Dublin. We identify and characterise the main noise sources as a function of space and time, comparing DAS signals with temporally overlapping broadband seismometer data. We discuss possible approaches to suppress incoherent noise along the cable for future shallow and deep geothermal monitoring, as well as imaging applications using coherent noise.

This research feeds into the European Union-funded Clean Energy Transition partnership project, GEOTWINS, which seeks to extend the state-of-the-art in modular geothermal digital twins, for improved deep geothermal imaging methodologies, drilling risk mitigation and to progress societal acceptance.

How to cite: Totten, E., Tary, J. B., and Chagas de Melo, B.: Distributed Acoustic Sensing (DAS) for Geothermal Applications: a Case Study Across Dublin City, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12365, https://doi.org/10.5194/egusphere-egu26-12365, 2026.

EGU26-12403 | Posters on site | SM3.4

Railway Distributed Acoustic Sensing data as an aid to earthquake monitoring in northernmost Sweden 

Björn Lund, Matti Rantatalo, Myrto Papadopoulou, Michael Roth, and Gunnar Eggertsson

The Swedish Transport Administration (STA) currently monitors the railway between Kiruna and the Swedish-Norwegian border with Distributed Acoustic Sensing (DAS), a distance of approximately 130 km. In collaboration with STA and Luleå University of Technology, the Swedish National Seismic Network (SNSN) has established data transmission on a request basis from the interrogator. As the railway crosses the Pärvie fault, the largest known, and still very active, glacially triggered fault, we hope to significantly improve detection and analysis of small earthquakes on that section of the fault. In this presentation we will show how we define low noise sections of the cable, using local and teleseismic events, and then use these as individual seismic stations. Over the 130 km, as the railway winds its way across the mountains, the cable generally runs in directions from N-S via NW-SE to W-E, providing many possible incidence directions. We discuss the technicalities of the data sharing, the existing metadata problems, how the DAS data is analyzed and incorporated into the routine processing at SNSN.

How to cite: Lund, B., Rantatalo, M., Papadopoulou, M., Roth, M., and Eggertsson, G.: Railway Distributed Acoustic Sensing data as an aid to earthquake monitoring in northernmost Sweden, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12403, https://doi.org/10.5194/egusphere-egu26-12403, 2026.

EGU26-12609 | ECS | Orals | SM3.4

Understanding fiber optic sensitivity to a wavefield: A framework to separate site amplification from orientation effects 

Olivier Fontaine, Andreas Fichtner, Thomas Hudson, Thomas Lecocq, and Corentin Caudron

Interpreting amplitudes in Distributed Acoustic Sensing (DAS) data is challenging because the recorded signal is influenced by multiple factors.

To differentiate the impact of fiber orientation from site effects, we develop expressions of axial strain for different body wave polarizations. These expressions consider a linear fiber segment with any orientation in space. From these we explore array geometry properties and the potential of the DAS transfer function as a polarization filter. This last property arises from the polarity inversion characteristic of shear waves and the averaging nature of the gauge length. If the gauge length is set to be a loop instead of a linear segment then the DAS will average all azimuth for a horizontal loop, canceling SH waves. For a vertical loop, all dips are averaged canceling SV waves traveling within the loop plane. These results could reflect a link between DAS and rotational seismology. 

From these transfers functions, we develop a low-cost forward model based on ray theory that predicts amplitude recorded in a DAS array. Differences in amplitude between the modeled and observed wavefields relate to local site amplification from which, we create an amplitude correction factor. We evaluated this method using active seismic experiments from the PoroTomo dataset, successfully identifying regions with anomalous high amplitude responses consistent with the recordings following a magnitude 4.3. 

The results, together with the main elements of our approach, are transferable in many new sensing strategies, including optimization of fiber deployment geometry, generations of synthetic data and the acceleration and improvement of existing location methods through DAS-specific amplitude and phase corrections.
In summary, by exploiting the known directional sensitivity of DAS, we draw new insights from amplitude variations along the fiber array, treating energy loss as equally informative as energy gain in interpreting the wavefield. 

How to cite: Fontaine, O., Fichtner, A., Hudson, T., Lecocq, T., and Caudron, C.: Understanding fiber optic sensitivity to a wavefield: A framework to separate site amplification from orientation effects, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12609, https://doi.org/10.5194/egusphere-egu26-12609, 2026.

EGU26-12675 | ECS | Orals | SM3.4

Strategies and Challenges in Applications of DAS-based Earthquake Early Warning Systems 

Claudio Strumia, Gaetano Festa, Alister Trabattoni, Diane Rivet, Luca Elia, Francesco Carotenuto, Simona Colombelli, Antonio Scala, Francesco Scotto di Uccio, and Anjali Suresh

Distributed Acoustic Sensing (DAS) transforms fiber-optic cables into ultra-dense strainmeter arrays, providing spatially and temporally continuous earthquake recordings. While its potential for offline seismic characterization is increasingly recognized, a key application of this sensing paradigm is real-time monitoring for Earthquake Early Warning (EEW). The use of existing fiber-optic infrastructures allows for sensing cables located close to seismogenic sources, such as offshore subduction zones, potentially extending the lead time of issued alerts. DAS deployments within Near Fault Observatories further provide dense spatial coverage of epicentral areas, favouring the rapid extraction of robust source information.

The application of DAS to EEW – alone or as a complement to standard accelerometers - has been recently explored, specifically focusing on the estimate of earthquake magnitude from the first seconds of recorded data. Existing approaches rely either on conversion strategies to ground-motion proxies or on direct analysis in the strain-rate domain. However, both the robustness of different conversion strategies and the selection of the most informative physical quantity for early magnitude estimation are not yet consolidated. In offshore environments, additional complexity arises from fiber-optic cables deployed on sediments, where strong converted phases often dominate early waveforms and hinder the direct P-wave signal traditionally used for EEW.

In this work, we analyse earthquakes recorded by the ABYSS network, supported by the ERC – starting program, consisting of 450 km of offshore telecommunication cables deployed along the Chilean subduction trench and interrogated by three DAS units. At this high-seismicity testbed, we develop a strategy for fast magnitude estimation with DAS. We show that converted Ps phases preceding S-wave arrivals carry significant information on earthquake magnitude. Furthermore, we investigated whether the use of time and space-integrated observables on DAS recordings can enhance the predictive power of amplitudes from the first seconds of seismic signals.

Finally, we assess the performance of a DAS-based EEW, grounded on the software PRESTo (Satriano et al., 2011). Using moderate-to-large offshore Chilean earthquakes, we highlight potential and limitations of DAS in regions with sparse conventional instrumentation. Complementary analyses using data from the Irpinia Near Fault Observatory demonstrate the benefits of jointly exploiting DAS and traditional seismic stations within dense monitoring networks, confirming the applicability of DAS-based EEW systems across different tectonic settings.

How to cite: Strumia, C., Festa, G., Trabattoni, A., Rivet, D., Elia, L., Carotenuto, F., Colombelli, S., Scala, A., Scotto di Uccio, F., and Suresh, A.: Strategies and Challenges in Applications of DAS-based Earthquake Early Warning Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12675, https://doi.org/10.5194/egusphere-egu26-12675, 2026.

EGU26-13083 | ECS | Orals | SM3.4

Long range Coherent-Optical Frequency Domain Reflectometry for large scale distributed sensing 

Debanjan Show, Biplab Dutta, Maël Abdelhak, Olivier Lopez, Adèle Hilico, Anne Amy-Klein, Christian Chardonnet, Paul-Eric Pottie, and Etienne Cantin

Fig. 1: Map of the REFIMEVE network (green links) and its connection to European links.

In recent years, significant technological progress has demonstrated the feasibility of using the long distance fiber optic links as large scale distributed networks for environmental sensing [1]. Optical fibers are inherently sensitive to external perturbations: their mechanical structure responds to strain, while the light propagating within them undergoes measurable intensity and phase variation when subjected to vibration or seismic waves. A notable example is the French national research infrastructure REFIMEVE [2], which distributes ultrastable time and frequency references across more than 9000 km of fiber links connecting laboratories throughout France and Europe (see Fig. 1). The infrastructure has demonstrated strong potential for geophysical studies [3]. Applications such as earthquake detection, volcano monitoring, and environmental hazard surveillance are attracting increasing interest worldwide, particularly because they can leverage already existing fiber networks. In this context, the European project SENSEI (Smart European Networks for Sensing the Environment and Internet Quality) [4] aims to harness this potential by developing the next generation photonic technologies for detecting both natural phenomena, such as earthquakes, volcano activity, and anthropogenic events including construction activity or vehicular traffic.

Within this framework, one of our objectives is to develop a coherent optical frequency domain reflectometry (C-OFDR) [5]. Current systems are limited to approximately 100 km by the coherence length of the laser source.  Here, we take benefit from the low frequency noise laser source generated by REFIMEVE frequency reference in order to extend the sensing range. In our setup, the output of a low noise laser is frequency modulated and a fiber under test is studied in a Michelson interferometer configuration. By analyzing the Rayleigh backscattered signal along the fiber, the system enables detailed diagnostics of the fiber under test including the detection of localized fiber deformations, faulty connectors, attenuation variations, and disturbances induced by environmental vibrations. As a first demonstration, we tested a prototype over a long range fiber link made of laboratory spools extending up to 335 km. The system successfully identified the position of the optical amplifier and a PC connector placed at the end of the fiber with km scale spatial resolution. In addition, vibration induced perturbation was observed and is under study, highlighting the potential of this technique for seismic applications. In future work, we plan to deploy the C-OFDR system on the operational REFIMEVE fiber network to evaluate its performance under real field conditions. This approach positions C-OFDR as a powerful tool for telecommunication infrastructure monitoring and distributed geophysical sensing.  

References :

[1] G. Marra et al., Science 361 (2018), https://doi.org/10.1126/science.aat4458

[2] REFIMEVE, https://www.refimeve.fr/en/homepage/

[3] M. B. K. Tønnes, PhD Thesis (2022), https://hal.science/tel-03984045v1

[4] SENSEI, https://senseiproject.eu/

[5] C. Liang et al., IEEE Access. 9 (2021), DOI: 10.1109/ACCESS.2021.3061250

How to cite: Show, D., Dutta, B., Abdelhak, M., Lopez, O., Hilico, A., Amy-Klein, A., Chardonnet, C., Pottie, P.-E., and Cantin, E.: Long range Coherent-Optical Frequency Domain Reflectometry for large scale distributed sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13083, https://doi.org/10.5194/egusphere-egu26-13083, 2026.

EGU26-13151 | Orals | SM3.4

Fiber optic cables (DAS) for seismic event detection – An underground case study 

Vincent Brémaud and Colin Madelaine

Distributed Acoustic Sensing (DAS), leveraging existing fiber optic infrastructure, represents a groundbreaking advancement in seismic monitoring. By converting telecommunication cables into dense arrays of virtual sensors, DAS enables continuous spatial coverage and enhanced sensitivity to seismic waves in remote or logistically constrained environments. This capability positions DAS as a complementary or alternative tool to traditional seismic networks, offering cost-effective, low-maintenance solutions for geophysical research and hazard monitoring.

This study focuses on the Premise-2 experiment, conducted at the Low-Noise Underground Laboratory (https://www.lsbb.eu/) in Rustrel, France, a site renowned for its low seismic noise. The experiment integrates active and passive seismic acquisitions, capturing both ambient noise and controlled seismic signals to assess DAS’s ability to detect and characterize events. Multiple fiber optic cable types and installation methods (laid on the ground, with sand bags, buried, or structurally attached) are evaluated to determine their impact on signal sensitivity, spatial resolution, and measurement robustness.

This study provides critical insights into optimal DAS deployment configurations for seismological applications while highlighting the challenges posed by large-scale data acquisition. The research underscores the need for advanced algorithms and specific workflows to fully exploit DAS’s potential. To characterized the events, we have used a workflow using automatic P and S arrival phases. We filtered these arrivals with an associator to select only detections that could be linked to an event. Then we tried different location algorithms to get a complete workflow from the acquisition to the location of the events.

How to cite: Brémaud, V. and Madelaine, C.: Fiber optic cables (DAS) for seismic event detection – An underground case study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13151, https://doi.org/10.5194/egusphere-egu26-13151, 2026.

EGU26-13235 | ECS | Orals | SM3.4

Distributed Acoustic Sensing at the Engineering Scale: Experimental Insights from the PITOP Test Site 

Olga Nesterova, Luca Schenato, Alexis Constantinou, Thurian Le Dû, Fabio Meneghini, Andrea Travan, Cinzia Bellezza, Gwenola Michaud, Andrea Marzona, Alessandro Brovelli, Silvia Zampato, Giorgio Cassiani, Jacopo Boaga, and Ilaria Barone

The PITOP geophysical test site, operated by the Istituto Nazionale di Oceanografia e di Geofisica Sperimentale (OGS) in north-eastern Italy, provides a unique experimental environment for testing seismic acquisition technologies under realistic field conditions. Covering ~22,000 m², PITOP was established to support the development and validation of geophysical methods and instrumentation in both surface and borehole installations. Here, we evaluate PITOP’s potential for Distributed Acoustic Sensing (DAS) experiments, focusing on small-scale seismic measurements relevant to urban settings and engineering applications. 

Five boreholes with distinct purposes and instrumentation are available at the PITOP site, including a water well (PITOP1), two 400-m-deep wells associated with geosteering research (PITOP2 and PITOP3), a 150-m-deep borehole permanently equipped with optical fibre for DAS measurements (PITOP4), and a recently drilled well dedicated to geoelectrical surveys (PITOP5). The site also hosts a surface-deployed fibre-optic cable, containing both linear and helicoidal fibers, and about 20 3C seismic nodes. Finally, several seismic sources are available, which are a borehole Sparker Pulse, suitable for crosshole VSP configurations, and two surface vibratory sources, the IVI MiniVib T-2500, which can generate sweeps in the 10–550 Hz frequency range, and the ElViS VII vibrator, designed for frequencies between 20 and 220 Hz.

We conducted three dedicated experiments:  (i) cross-hole measurements with sources in PITOP3 at depths of 10, 50, 75, and 100 m, and DAS recording in PITOP4; (ii) a vertical seismic profiling (VSP) survey using the MiniVib source close to the well head with DAS recording in PITOP4; and  (iii) recordings of the seismic wavefield generated by P- and S-wave vibratory sources using surface DAS arrays in linear and helicoidal configurations, together with co-located 3D geophones for comparison.

DAS data were acquired with multiple gauge lengths and acquisition settings. The resulting datasets enable a systematic evaluation of acquisition parameters selection and highlight processing strategies required for different DAS configurations. They provide a valuable basis for assessing optimal DAS acquisition strategies for small-scale seismic applications and for defining processing workflows adapted to diverse source and receiver geometries.

The present study is being carried out within the framework of the USES2 project, which receives funding from the EUROPEAN RESEARCH EXECUTIVE AGENCY (REA) under the Marie Skłodowska-Curie grant agreement No 101072599.

This research has been supported by the Interdepartmental Research Center for Cultural Heritage CIBA (University of Padova) with the World Class Research Infrastructure (WCRI) SYCURI—SYnergic strategies for CUltural heritage at RIsk, funded by the University of Padova.

How to cite: Nesterova, O., Schenato, L., Constantinou, A., Le Dû, T., Meneghini, F., Travan, A., Bellezza, C., Michaud, G., Marzona, A., Brovelli, A., Zampato, S., Cassiani, G., Boaga, J., and Barone, I.: Distributed Acoustic Sensing at the Engineering Scale: Experimental Insights from the PITOP Test Site, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13235, https://doi.org/10.5194/egusphere-egu26-13235, 2026.

EGU26-13315 | ECS | Orals | SM3.4

Deep Learning-Based Earthquakes Localization at Campi Flegrei via Distributed Acoustic Sensing 

Miriana Corsaro, Léonard Seydoux, Gilda Currenti, Flavio Cannavò, Simone Palazzo, Martina Allegra, Philippe Jousset, Michele Prestifilippo, and Concetto Spampinato

The current phase of unrest of the Campi Flegrei caldera (Italy), one of the most dangerous volcanic complexes in the world, requires increasingly rapid and high-resolution seismic monitoring solutions. In this context, Distributed Acoustic Sensing (DAS) has recently emerged as a highly innovative technology, enabling existing fiber-optic cables to be repurposed into ultra-dense seismic arrays capable of sampling the seismic wavefield with unprecedented spatial resolution.

In this study, we present a new earthquake-localization method that uses automatically identified P- and S-wave arrivals on DAS data to localize seismic events. Employing Transformer-based architectures designed to process DAS's high-dimensional strain data, our approach simultaneously estimates key source parameters, including hypocentral location, magnitude, and origin time. A comparative analysis against the official seismic catalogue reveals minimal residuals, validating the model's robustness. 

The model therefore represents a significant advancement, as it enables reliable earthquake localization in extremely short time frames using exclusively automatically picked data, while simultaneously overcoming the computational bottlenecks typical of traditional processing workflows. As a result, this methodology establishes a new benchmark for real-time monitoring of magmatic and hydrothermal systems, substantially contributing to improved seismic hazard assessment.

How to cite: Corsaro, M., Seydoux, L., Currenti, G., Cannavò, F., Palazzo, S., Allegra, M., Jousset, P., Prestifilippo, M., and Spampinato, C.: Deep Learning-Based Earthquakes Localization at Campi Flegrei via Distributed Acoustic Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13315, https://doi.org/10.5194/egusphere-egu26-13315, 2026.

EGU26-13382 | ECS | Posters on site | SM3.4

Towards ambient noise tomography on long telecommunication cables: using DAS for characterisation of the seismo-acoustic soundscape in the Atlantic Ocean and Irish Sea 

Rosa Vergara González, Nicolas Luca Celli, Christopher J. Bean, Marco Ruffini, and Örn Jónsson

The oceans are a noisy place, where ships, waves, storms, currents, earthquakes and marine wildlife all leave their own seismo-acoustic signatures. Fibre sensing has the potential to allow researchers to utilise the thousands of sea-bottom telecommunication fibre-optic cables spread across the globe, and with them, we can record, characterise and monitor these signals from up close. However, at present sensing equipment limitations, lack of established fibre-sensing workflows and access to cables severely limit the use of this technology in the seas.

Here, we present and analyse Distributed Acoustic Sensing (DAS) data newly recorded on long, telecom fibre-optic cables offshore through the east and west coasts of Ireland. The availability of these two different datasets allows us to compare different environments and physical phenomena across a large region. The eastern cable covers 118 km from Dublin, Ireland to Holyhead, Wales with 36 days of data recorded in Spring 2025, while the western one reaches 72 km offshore from Galway, with 60 days of data in Autumn 2025. These datasets form part of a much larger compendium, including data from approximately 300km of onshore fibre-optic cables between both shores. Thanks to the large cable lengths and long recording times, we observe a plethora of short-lived, high frequency signals such as ships, anthropogenic noise, and local earthquakes, as well as long-wavelength, long-period signals such as ocean storms and microseisms, tides, and teleseismic events.

To characterise observations in these noisy environments, we compare our observations with nearby land seismic stations and weather records to track storm systems and wave height. We identify and separate the different seismic and acoustic sources observed, resulting in a preliminary catalogue of dominant signal types observed along the cables. The results are utilised to highlight the differences between the two marine environments and separate marine, seismic and anthropic transient signals from ambient noise. This is key to improve our understanding of ocean processes and to build datasets suitable for deep Earth sensing through Ambient Noise Tomography. While our focus is seismic, characterising marine seismic and acoustic phenomena is key in applications well beyond this field, from telecommunication fibre cable safety, to marine biology and oceanographic applications.

How to cite: Vergara González, R., Celli, N. L., Bean, C. J., Ruffini, M., and Jónsson, Ö.: Towards ambient noise tomography on long telecommunication cables: using DAS for characterisation of the seismo-acoustic soundscape in the Atlantic Ocean and Irish Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13382, https://doi.org/10.5194/egusphere-egu26-13382, 2026.

EGU26-13416 | ECS | Posters on site | SM3.4

Temperature and strain monitoring in Reykjanes geothermal field, Iceland, using quasi-distributed fiber-optic sensing 

Julien Govoorts, Corentin Caudron, Jiaxuan Li, Haiyang Liao, Christophe Caucheteur, Yesim Çubuk-Sabuncu, Halldór Geirsson, Vala Hjörleifsdóttir, Kristín Jónsdóttir, and Loic Peiffer

Since December 2023 and after 800 years of inactivity, recurrent volcanic eruptions are taking place at the Svartsengi volcanic system indicating the start of a new volcanic cycle. In contrast, the Reykjanes volcanic system, located to the west of Svartsengi, has remained dormant since the 13th century.  The Reykjanes geothermal area, in particular the Gunnuhver geothermal field, is located at the westernmost end of the Reykjanes Peninsula. This geothermal area is associated with the upflow of seawater-derived hydrothermal fluids and characterized by numerous geothermal features, including steam vents and steam-heated mud pools.

Since October 2022, this geothermal field has been continuously monitored using a variety of technologies to record parameters such as soil temperature, strain and electrical resistivity. The present study focuses primarily on the parameters gathered from August 2024 using the Fiber Bragg Grating (FBG) technology, a point fiber-optic sensing approach. This technique utilizes wavelength-division multiplexing, meaning the fiber is capable of transmitting information at distinct wavelengths. Consequently, given that each FBG possesses its own wavelength, the fiber is transformed into a cost-effective and versatile quasi-distributed sensor.

Over the course of a year, the FBG interrogator deployed on-site has measured the wavelength changes at a sampling frequency ranging from 0.4Hz to 1Hz. These changes were recorded from 24 different temperature probes and 8 strain sensors both buried in-ground throughout the geothermal field. Most of the temperature sensors were installed in areas of the soil where no geothermal surface manifestation was present. These sensors recorded temperature changes primarily driven by variations in atmospheric temperature. In contrast, the remaining sensors were directly located in altered areas or close to steam vents. These sensors exhibit clear cooling patterns due to precipitation but do not show temperature changes that can be attributed to the eruption cycle. Additionally, the FBG temperature sensors allow the identification of fiber sections that are coupled to air temperature fluctuations along a telecom fiber deployed a few hundred meters north and monitored by a Distributed Acoustic Sensing (DAS) interrogator.

In addition to the temperature probes, the strain sensors have recorded signals ranging from periodic dynamic strain changes attributed to industrial processes, to static strain changes assigned to crustal deformation. On April 1, 2025, a volcanic eruption occurred in the Svartsengi volcanic system, resulting in strain variations observed 15 kilometers away from the eruption site using FBG and low-frequency components of DAS recordings. These variations were also observed in strain measurements obtained from permanent network GNSS stations. This experiment demonstrates the capacity and reliability of the FBG technology for monitoring temperature changes and deformation signals in an active geothermal environment.

How to cite: Govoorts, J., Caudron, C., Li, J., Liao, H., Caucheteur, C., Çubuk-Sabuncu, Y., Geirsson, H., Hjörleifsdóttir, V., Jónsdóttir, K., and Peiffer, L.: Temperature and strain monitoring in Reykjanes geothermal field, Iceland, using quasi-distributed fiber-optic sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13416, https://doi.org/10.5194/egusphere-egu26-13416, 2026.

EGU26-13921 | ECS | Orals | SM3.4

Seismic Characterisation of an Arctic Glacier 

Tora Haugen Myklebust, Martin Landrø, Robin André Rørstadbotnen, and Calder Robinson

In recent years, Distributed Acoustic Sensing (DAS) has emerged as a cost-effective seismic monitoring tool for cryosphere research. Compared to conventional geophone arrays, the DAS system is compact, easy to transport, and can be rapidly deployed over large distances in glaciated environments.

Previous studies have demonstrated that DAS is a useful tool for ice-sheet imaging and monitoring glacier dynamics. For example, using borehole DAS in conjunction with surface explosives (e.g., Booth et al., 2022; Fitchner et al., 2023) or passive recordings using surface DAS (e.g., Walter et al., 2020; Gräff et al, 2025). Significant progress has been made in applying surface DAS for active marine subsurface imaging (e.g., Pedersen et al., 2022; Raknes et al., 2025). We extend this approach to active englacial and subglacial imaging on Slakbreen, Svalbard.

During a multi-geophysical field campaign in March 2025, we acquired seismic data using surface explosives along an approximately 2 km fibre co-located with a vertical-component geophone array. We process different reflected modes (PP and PS) recorded on the fibre and benchmark the imaging results against the equivalent PP-image from the geophone array. We evaluate differences in wavefield sensitivity across the three datasets and we will present how these can be used to characterise the state of the cryosphere and deeper sedimentary successions.

Despite the relative immaturity of DAS for glacier imaging and current limitations of the processing workflow, our results clearly establish surface DAS as a viable monitoring tool for seismic imaging of the cryosphere and as a potential enabler of large-scale seismic monitoring of glaciers and the subsurface.

 

References:

Booth, A. D., P. Christoffersen, A. Pretorius, J. Chapman, B. Hubbard, E. C. Smith, S. de Ridder, A. Nowacki, B. P. Lipovsky, and M. Denolle, 2022, Characterising sediment thickness beneath a greenlandic outlet glacier using distributed acoustic sensing: preliminary observations and progress towards an efficient machine learning approach: Annals of Glaciology, 63(87-89):79–82.                                                                                                                                                   

Fichtner, A., C. Hofstede, L. Gebraad, A. Zunino, D. Zigone, and O. Eisen, 2023, Borehole fibre-optic seismology inside the northeast greenland ice stream: Geo-physical Journal International, 235(3):2430–2441.

Gräff, D., B. P. Lipovsky, A. Vieli, A. Dachauer, R. Jackson, D. Farinotti, J. Schmale, J.-P. Ampuero, E. Berg, A. Dannowski, et al., 2025, Calving-driven fjord dynamics resolved by seafloor fibre sensing: Nature, 644(8076):404–412.

Pedersen, A., H. Westerdahl, M. Thompson, C. Sagary, and J. Brenne, 2022, A north sea case study: Does das have potential for permanent reservoir monitoring? In Proceedings of the 83rd EAGE Annual Conference & Exhibition, pages 1–5. European Association of Geoscientists & Engineers.

Raknes, E. B., B. Foseide, and G. Jansson, 2025, Acquisition and imaging of ocean-bottom fiber-optic distributed acoustic sensing data using a full-shot carpet from a conventional 3d survey: Geophysics, 90(5):P99–P112.

Walter, F., D. Gräff, F. Lindner, P. Paitz, M. Köpfli, M. Chmiel, and A. Fichtner,2020, Distributed acoustic sensing of microseismic sources and wave propagation in glaciated terrain: Nature communications, 11(1):2436.

How to cite: Myklebust, T. H., Landrø, M., Rørstadbotnen, R. A., and Robinson, C.: Seismic Characterisation of an Arctic Glacier, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13921, https://doi.org/10.5194/egusphere-egu26-13921, 2026.

EGU26-14230 | ECS | Orals | SM3.4

Unveiling type of fiber and coupling conditions effects on geophysical DAS measurements, results from underground experiments 

Vanessa Carrillo-Barra, Diego Mercerat, Vincent Brémaud, Anthony Sladen, Olivier Sèbe, Amaury Vallage, and Jean-Paul Ampuero

Optical fiber measurements have been demonstrated to be useful in assessing geophysical near-surface parameters and in detecting seismological events in newly accessible regions (e.g. cities, ocean floor, highways) by leveraging the existing fiber-optic infrastructure. In particular, laser interferometry performed with DAS systems (Distributed Acoustic Sensing) allows measuring the cable axial strain related to passing seismo-acoustic waves, at any point along the fiber and over tens of kilometers of cable.

However, compared to traditional seismic sensors the instrumental response of DAS remains unclear, and there is in particular a critical need to better understand how the measurements are influenced by the nature of the fiber optic cable and its coupling to the ground or medium under study. To explore this question, we present results from two active seismic campaigns carried out in the low-noise  underground tunnel LSBB (Laboratoire Souterrain à Bas Bruit), in southeastern France.

We recorded multiple active sources (TNT detonations and hammer shots) by a 10km and 2km long underground optical fiber set-ups and with conventional seismic sensors as well. We tested along both campaigns different optical fiber cable designs and different types of coupling conditions (sealed, sandbags weighted, freely posed) installed in parallel. This experimental setup provides a unique opportunity to examine in detail and quantify the possible variations in the strain signals recovered from DAS data.

Preliminary observations reveal significant discrepancies in the recorded data depending on the coupling conditions. The characteristics of the deployed source result in a signal that is primarily concentrated in the high-frequency range, for which the sealed fiber does not necessarily exhibit a significantly improved response. Additionally, the acoustic wave generated by the hammer-shot echo, propagating through the air, is strongly amplified in all cables covered by sandbags. We propose that the sandbags increase the interaction area between that signal and the cables, thereby enhancing reverberation.

Furthermore, we observe systematic differences in the maximum amplitudes recorded by the different cables tested, with the telecom cable consistently exhibiting lower amplitudes than other specialized cables, suggesting a lower sensitivity. However, this reduction is relatively modest, and when combined with the substantially lower cost of telecom cables, indicates that they remain a cost-efficient alternative for certain experiments. Additional observations and detailed analyses from this study will be presented.

 

Keywords: Coupling, fiber optics, DAS measurements, strain rate, active seismic, LSBB.

How to cite: Carrillo-Barra, V., Mercerat, D., Brémaud, V., Sladen, A., Sèbe, O., Vallage, A., and Ampuero, J.-P.: Unveiling type of fiber and coupling conditions effects on geophysical DAS measurements, results from underground experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14230, https://doi.org/10.5194/egusphere-egu26-14230, 2026.

EGU26-15142 | ECS | Orals | SM3.4

Toward Global-Scale Submarine Fiber Sensing: Early Results from Multispan DAS at the OOI Regional Cabled Array 

Zoe Krauss, Bradley Lipovsky, Mikael Mazur, William Wilcock, Nicolas Fontaine, Roland Ryf, Alex Rose, William Dientsfrey, Shima Abadi, Marine Denolle, and Renate Hartog

A recently developed multispan distributed acoustic sensing (multispan-DAS) technique from Nokia Bell Labs enables strain measurements along submarine fiber-optic cables across multiple repeater-separated spans. By leveraging the high-loss loopback couplers within optical repeaters, this technique overcomes the long-standing limitation of conventional DAS to the first span of a repeated cable, typically < 100 km offshore. Dense, continuous arrays of seafloor strain sensors can now extend to hundreds or thousands of kilometers. This technique has been used to successfully record the 2025 M8.8 Kamchatka earthquake and tsunami at teleseismic range with a spatial resolution of ~100 m across 4400 km of a repeated submarine cable.

In November 2025, the multispan-DAS system from Nokia Bell Labs was deployed for three months on both repeated submarine cables of the Ocean Observatories Initiative Regional Cabled Array (OOI RCA) offshore Oregon. The deployment traverses the Cascadia subduction zone forearc and extends approximately 500 km offshore to Axial Seamount. During this period, the first span of the southern cable was simultaneously interrogated using a multiplexed conventional DAS unit, while data continued to stream from co-located cabled seismometers, hydrophones, and other oceanographic instruments on the OOI RCA.

The multispan-DAS system recorded a regional earthquake beyond the first repeater of both cables during testing as well as the ambient seafloor seismic wavefield, demonstrating sensitivity to a broad range of seismic, oceanographic, and acoustic signals. These observations provide a unique opportunity to directly compare multispan-DAS measurements with conventional DAS and established seafloor instrumentation across a large spatial extent. The resulting dataset will be publicly released following documentation and quality control. We will present preliminary results characterizing the noise floor, sensitivity, and signal fidelity of multispan-DAS relative to co-located sensors, and examine the consistency of observed seismic and oceanographic signals across measurement modalities. These results will highlight the potential of multispan-DAS for applications including routine earthquake monitoring, earthquake early warning, and broader seafloor observation, and represent an important step toward establishing this technique as a new tool for the seismological and oceanographic communities.

How to cite: Krauss, Z., Lipovsky, B., Mazur, M., Wilcock, W., Fontaine, N., Ryf, R., Rose, A., Dientsfrey, W., Abadi, S., Denolle, M., and Hartog, R.: Toward Global-Scale Submarine Fiber Sensing: Early Results from Multispan DAS at the OOI Regional Cabled Array, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15142, https://doi.org/10.5194/egusphere-egu26-15142, 2026.

EGU26-15227 | Posters on site | SM3.4

Enhancing Earthquake Location in the Central Apennines (Italy): A Hybrid Approach Combining Arrivals from Line-Sensor Telecom Fiber Interferometry and Traditional Point-sensors 

Diana Latorre, Cecilia Clivati, André Herrero, Anthony Lomax, Raffaele Di Stefano, Simone Donadello, Aladino Govoni, Maurizio Vassallo, and Lucia Margheriti

The integration of existing telecommunication fiber-optic infrastructure into seismic monitoring networks offers a transformative opportunity to densify observations in seismically active regions. We present the results of a multi-year monitoring experiment (2021–2026) utilizing a 39-km telecom fiber link from the Italian telecommunication company Open Fiber between Ascoli Piceno and Teramo in the Central Apennines, Italy. The system employs an ultra stable laser to measure seismic-induced deformation of the fiber, operating on a dedicated wavelength in coexistence with commercial data traffic.

A significant challenge in utilizing fiber-optic data for earthquake location is the transition from traditional point-sensor geometry to distributed sensing. To address this, we implemented a hybrid localization approach using a modified version of the NonLinLoc (NLL) algorithm. We move beyond traditional discrete measurements (point sensors) by treating the cable as a continuous "line sensor." Following the NLL algorithm, the most effective strategy is translating both point and line geometries into a unified framework of 3D travel-time maps. Once the sensors are translated into these maps, their combined use for location becomes independent of the sensor type, allowing for a seamless merging of traditional seismic station data and fiber-optic pickings. 

We applied this methodology to the real seismic catalog recorded from the fiber's installation in mid 2021 until January 2026 in the Ascoli-Teramo area, a region where the Italian seismic network is relatively sparse. Specifically, we analyzed signals from: 1) several small seismic sequences occurring at short distances (up to approximately 20 km) from the fiber cable, including the Civitella del Tronto (TE) sequence that followed a Mw 3.9 event (September 22, 2022); and 2) more distant earthquakes (ranging from approximately 20 to 50 km from the fiber) with local magnitudes exceeding ML 2.5, distributed along the Central Apennines axis. For events where the fiber signal allowed for the correct identification of P- and S-wave arrival times, we applied the NLL algorithm using the integrated network. In this work, we present several of these examples and associated tests to discuss how the inclusion of fiber-derived arrival times can provide further hypocentral constraints. This study aims to highlight the scalability of fiber interferometry combined with non-linear inversion as a robust tool for seismic surveillance in populated and high-risk tectonic environments.

How to cite: Latorre, D., Clivati, C., Herrero, A., Lomax, A., Di Stefano, R., Donadello, S., Govoni, A., Vassallo, M., and Margheriti, L.: Enhancing Earthquake Location in the Central Apennines (Italy): A Hybrid Approach Combining Arrivals from Line-Sensor Telecom Fiber Interferometry and Traditional Point-sensors, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15227, https://doi.org/10.5194/egusphere-egu26-15227, 2026.

EGU26-16522 | ECS | Posters on site | SM3.4

Detecting Microseismic Events Using Cross-Fault Borehole DAS 

Chih-Chieh Tseng, Hao Kuo-Chen, Li-Yu Kan, Sheng-Yan Pan, Wei-Fang Sun, Chin-Shang Ku, and Ching-Chou Fu

Microseismic events account for the majority of seismicity, however, sparse station spacing hinders the detection of such small events. In recent decades, distributed acoustic sensing (DAS) has shown its power to provide a denser spatial sampling in an array sense, to resolve weak signals that are often missed by conventional seismometers. In eastern Taiwan, the Chihshang fault plays a key role in accommodating deformation along the Longitudinal Valley fault system, where frequent small earthquakes and fault creep occur. In this study, we develop a new workflow for microseismic event detection by integrating borehole DAS data with the deep-learning-based automatic phase picking model PhaseNet. An event is declared when more than 75% of channels record P-wave picks and more than 30% record S-wave picks within a 1-s time window. We analyzed three months of DAS data from March to July 2025. As a result, we identified approximately twice as many events as those reported in a deep-learning-based earthquake catalog constructed using only surface seismic stations. These results suggest that borehole DAS provides an effective complementary constraint for detecting earthquake-generated wave trains. This processing workflow can significantly improve the detection capability for microseismic events, leading to higher seismic catalog completeness and finer fault structure near the Chihshang region.

How to cite: Tseng, C.-C., Kuo-Chen, H., Kan, L.-Y., Pan, S.-Y., Sun, W.-F., Ku, C.-S., and Fu, C.-C.: Detecting Microseismic Events Using Cross-Fault Borehole DAS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16522, https://doi.org/10.5194/egusphere-egu26-16522, 2026.

EGU26-16913 | ECS | Posters on site | SM3.4

Cross-validating Distributed Acoustic Sensing and Seismic Records for Shallow Ground Motion and Near-Surface Properties 

Marco Pascal Roth, Xiang Chen, Gian Maria Bocchini, and Rebecca M Harrington

Distributed Acoustic Sensing (DAS) offers dense spatial sampling of ground motion and has the potential to perform detailed seismic monitoring and constrain shallow velocity structure. In this study, we analyze ground motion recorded by broadband seismometers and a fiber-optic interrogator of two shallow tectonic earthquakes in the Roerdalen region (The Netherlands–Germany border) with local magnitudes ML 2.2 (2025-09-09) and ML 1.9 (2025-09-15) and hypocentral depths of ~15 km to quantify the differences in sensitivity and magnitude estimates from each type of instrumentation. The Distributed Acoustic Sensing (DAS) recordings consist of ground strain sampled at 250 Hz on a 30 km telecommunications dark-fiber with a channel spacing of 5 m and a gauge length of 50 m. Seismometer recordings consist of ground velocity sampled at 100 Hz on a Trillium Compact 20 s seismometer that has a flat frequency response up to ~100 Hz. Both types of sensors recorded the earthquakes with a minimum epicentral distance of ~20 and 10 km, respectively. We will present results showing the differences in frequency sensitivity, conversions to ground displacement, and estimated magnitudes, as well as an interpretation of differences based on the shallow ground velocity. 

We first convert DAS recordings that are initially measured in strain to ground displacement using a semblance-based approach, as well conventional seismic recordings initially recorded in velocity. We make a quantitative comparison of waveform characteristics, including amplitude-frequency dependence and its variability in space for point-wise seismic sensor measurements vs. DAS measurements. We will present an interpretation of the results based on the context of geological setting to identify spatial variations that cannot be resolved by the sparse seismic network alone. As DAS measurements reveal significant lateral variability in ground motion amplitudes that suggest a strong influence of near-surface conditions (density) and/or local coupling effects, we will also quantify the relative influence of each using a comparison of strain and converted ground displacement. In addition, we explore approaches to estimate earthquake magnitude from DAS data by relating observed strain amplitudes to ground-motion parameters derived from the co-located seismometer. Preliminary results suggest that DAS-based observations capture the relative scaling between the two events and show promise for magnitude estimation when calibrated against conventional seismic sensors. Our findings demonstrate the value of DAS for high-resolution observations of near surface properties and their influence on earthquake waveforms.  They also highlight the potential of DAS to complement existing seismic networks for monitoring small-magnitude earthquakes.  

How to cite: Roth, M. P., Chen, X., Bocchini, G. M., and Harrington, R. M.: Cross-validating Distributed Acoustic Sensing and Seismic Records for Shallow Ground Motion and Near-Surface Properties, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16913, https://doi.org/10.5194/egusphere-egu26-16913, 2026.

EGU26-17223 | ECS | Orals | SM3.4

Reimagining Seismic Array Processing with Fibre-Optic DAS: The NORFOX Array 

Antoine Turquet, Andreas Wuestefeld, Alan Baird, Kamran Iranpour, and Ravn Rydtun

NORFOX is a purpose-built fibre-optic Distributed Acoustic Sensing (DAS) installation located in southeastern Norway, approximately 150 km north of Oslo. Beyond its primary function of monitoring earthquakes and explosions, the system captures a broad range of other signals, including aircraft, thunder, and atmospheric phenomena. A key advantage of NORFOX is its overlap with the co-located NORES seismometer array, which enables direct calibration of DAS measurements against conventional seismic recordings and supports method development under well-constrained ground-truth conditions. In this contribution, we introduce the NORFOX infrastructure and array layout, discuss key design choices, and summarize practical strengths and limitations using representative examples.

NORFOX is additionally equipped with all-sky cameras operated by Norsk Meteor Nettverk for meteor monitoring, which also capture nearby lightning activity. Lightning locations provide independent timing and spatial context that help interpretation coincident acoustic signatures observed on the fibre. Together with weather information, noise-floor characterization, and optical monitoring, these observations provide a benchmark dataset for both existing and future DAS installations and calibration

We also present in-house approaches to reduce noise, understanding signals, strategies on managing data volumes and edge-computing. Furthermore, we show and interpret signals from nearby quarry blasts, regional earthquakes, thunderstorms, and aircraft. Finally, we demonstrate and evaluate DAS array-processing methodologies for earthquake and explosion monitoring at NORFOX. Overall, dedicated research fibre arrays such as NORFOX provide a controlled environment to develop, benchmark, and calibrate DAS-based monitoring workflows in combination with co-located seismic instrumentation.

How to cite: Turquet, A., Wuestefeld, A., Baird, A., Iranpour, K., and Rydtun, R.: Reimagining Seismic Array Processing with Fibre-Optic DAS: The NORFOX Array, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17223, https://doi.org/10.5194/egusphere-egu26-17223, 2026.

EGU26-17496 | ECS | Orals | SM3.4

Privacy Concerns of DAS: Eavesdropping using Neural Network Transcription 

Jack Lee Smith, Karen Lythgoe, Andrew Curtis, Harry Whitelam, Dominic Seager, Jessica Johnson, and Mohammad Belal

Distributed acoustic sensing (DAS) has transformed geophysical, environmental, and infrastructure monitoring. However, the increasing bandwidth and sensitivity of modern interrogators now extend into the audio range, introducing a material privacy risk. Here we demonstrate, through in-situ experiments on live fibre deployments, that human speech, music, and other acoustic signals can be under certain acquisition conditions.

We show that intelligible speech can be accurately recovered and automatically transcribed using neural networks. Experiments were conducted on both linear and spooled fibre geometries, deployed as part of an ongoing geophysical survey. We find that coiled layouts, which are common in access networks (e.g., slack loops or storage spools), exhibit enhanced sensitivity to incident acoustic waves relative to linear layouts. Modelling indicates this arises from increased broadside sensitivity and reduced destructive interference for longer wavelength acoustic fields over the gauge length. We systematically assess how acquisition parameters, such as source-fibre offset, influence signal‑to‑noise ratio, spectral fidelity, and speech intelligibility of recorded audio. We further show that neural network based denoising strategies improves intelligibility and fidelity of recorded audio, thereby exacerbating privacy concerns.

These findings demonstrate that appropriate interrogation of existing fibre infrastructure - including fibre‑to‑the‑premises links, smart-city infrastructure, and research cables – can function as pervasive, passive wide-area acoustic receivers, creating a pathway for inadvertent or malicious eavesdropping. We discuss practical mitigation strategies spanning survey design, interrogation configuration, and data governance, and argue that the incorporation of privacy‑by‑design into deployment and processing is crucial to leverage the unique benefits of DAS while managing emerging ethical and legal risks.

How to cite: Smith, J. L., Lythgoe, K., Curtis, A., Whitelam, H., Seager, D., Johnson, J., and Belal, M.: Privacy Concerns of DAS: Eavesdropping using Neural Network Transcription, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17496, https://doi.org/10.5194/egusphere-egu26-17496, 2026.

EGU26-17601 | Posters on site | SM3.4

Ambient signals analysis and cable coupling characterisation from a DAS experiment offshore South Brittany 

Florian Le Pape, Stephan Ker, Shane Murphy, Philippe Schnurle, Mikael Evain, Pascal Pelleau, Alexis Constantinou, and Patrick Jousset

As fibre-sensing measurements on submarine fibre optic cables become more widely used in geophysical studies, new challenges arise that demand a deeper understanding of the collected data. In particular, characterisation of cable coupling to the seafloor as well as the response of local sediment under the cables is needed for a better quantification of external physical phenomena by fibre-sensing measurements.

FiberSCOPE is a research project aiming to implement an intelligent seabed monitoring system for studies in seismology, oceanography and the positioning of acoustic manmade sources (ships, AUVs, etc.) using existing submarine fiber-optic cables. One of the main objectives of the project is to define tools for remote evaluation of fibre optic cable coupling with the seabed using both Brillouin Optical Time Domain Reflectometry (BOTDR) and Distributed Acoustic Sensing (DAS) measurements of ambient noise.

Within the project’s framework, passive and active seismic experiments were performed during March-April 2025 offshore south Brittany. The experiment included acquiring DAS measurements on the electro-optic cable connecting mainland France to Groix island, combined with the deployment of 10 seismic nodes near the cable. Preliminary results show that although ocean waves dominate the DAS signals, ocean wave induced microseisms events can be extracted as they fluctuate over the 18 days’ of the passive acquisition. Interestingly, despite the short distance covered by the offshore portion of the cable, spatial variations of those events are also observed and seem consistent between cable and nodes measurements. Finally, both ocean waves and microseism signals are used to further quantify the cable coupling with the seafloor and cable response connected to changes in seafloor structure.

How to cite: Le Pape, F., Ker, S., Murphy, S., Schnurle, P., Evain, M., Pelleau, P., Constantinou, A., and Jousset, P.: Ambient signals analysis and cable coupling characterisation from a DAS experiment offshore South Brittany, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17601, https://doi.org/10.5194/egusphere-egu26-17601, 2026.

EGU26-18270 | ECS | Posters on site | SM3.4

Assessing the Seismic Sensitivity on a Submarine Optical Fiber Link between Malta and Catania (Sicily, Italy) 

Daniele Caruana, Matthew Agius, André Xuereb, Cecilia Clivati, Simone Donadello, Kristian Grixti, and Irena Schulten

Submarine regions remain sparsely instrumented, limiting the spatial coverage of seismic monitoring in offshore environments. Recent studies have shown that optical fibers, including those actively used for telecommunications, can detect ground motion through laser interferometry. We present an ongoing evaluation of the seismic sensitivity of a 260 km optical fiber link between Malta and Catania, predominantly submerged in the Ionian Sea and continuously carrying internet traffic.

The optical-fiber recordings were analysed for signals corresponding to the arrival times of ~1500 earthquakes listed in the INGV catalogue between January 2023 and March 2025. The waveforms were manually inspected for seismic arrivals and compared to seismic data recorded on nearby land stations on Malta and Sicily. Earthquakes ranging from magnitude 1.4 to 7.9 originating from distance of 3 to 16,000 km were successfully observed. Each event was assigned a category according to signal clarity and confidence, ranging from clearly visible arrivals (category A) to non-detectable signals (category E). Preliminary results indicate that <10% of events fall into category A, 10-15% in category B, 20-25% in category C, 20-25% in category D, and >30% in category E, providing an initial characterisation of the optical-fiber cable’s sensitivity. While a majority of observations fall within lower quality categories (D-E), at least 35% of the analysed events remain robustly identifiable, highlighting the contribution of the submarine fiber to existing land-based seismic networks and extending observational coverage in submarine regions. The sensitivity of the fiber strongly depends on the earthquake magnitude-distance relationship, as expected. We compare our results with previously reported measurements on terrestrial fibers (Donadello, et al., 2024), and show that the Malta-Catania submarine cable can be a reliable new seismic tool for a submarine environment, although recording fewer high-confidence events than onshore systems.

Noise in the fiber exhibits correlations with wind and with daytime anthropogenic activity. This reduces the signal-to-noise ratio and limits the detectability of earthquakes with M<2. Ongoing data acquisition will further refine sensitivity estimates and improve the characterisation of the fiber’s seismic performance.

This study is part of the Horizon Europe–funded SENSEI project, which aims to transform fibre-optic communication networks into distributed sensors for detecting environmental and geophysical signals, improving monitoring and early warning across Europe (Project ID 101189545).

How to cite: Caruana, D., Agius, M., Xuereb, A., Clivati, C., Donadello, S., Grixti, K., and Schulten, I.: Assessing the Seismic Sensitivity on a Submarine Optical Fiber Link between Malta and Catania (Sicily, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18270, https://doi.org/10.5194/egusphere-egu26-18270, 2026.

EGU26-19501 | ECS | Posters on site | SM3.4

 Investigating subsea cable sensing for monitoring of marine life, detection of earthquakes and tsunamis with Research and Education network infrastructure 

Shima Ebrahimi, Layla Loffredo, Alexander van den Hil, and Richa Malhotra

Recent advances in fibre-optic sensing enable subsea telecommunication cables to function as large-scale, distributed environmental sensors. Techniques such as Distributed Acoustic Sensing (DAS), State of Polarisation (SOP), and interferometry transform optical fibres into continuous arrays capable of detecting seismic, acoustic, and environmental signals, offering a complementary, future-proof  approach to sparsely deployed subsea instruments. This study, conducted by SURF, the Dutch National Research and Education Network (NREN), assesses the feasibility of leveraging existing and future subsea fibre-optic network infrastructure for scientific sensing within the research ecosystem. The analysis is based on an extensive data collection effort, including 55 semi-structured interviews with international experts across geoscience, marine science, networking, and technology domains, as well as a targeted survey of research institutions, which received 20 responses from 42 invited experts. Results indicate that dry-plant sensing techniques are sufficiently mature for near-term applications, with DAS enabling kilometre-scale seismic and acoustic monitoring, while SOP and interferometry support long-range sensing over thousands of kilometres. Wet-plant approaches, including SMART cables and Fiber Bragg Grating sensors, provide high-precision measurements at extreme depths but remain limited to new cable deployments due to cost and coordination requirements. Strong alignment is observed with current needs in seismology and geophysics, particularly for offshore seismic monitoring and subsurface deformation studies, while applications in oceanography and marine biology remain exploratory. Data volume, standardisation, and real-time processing emerge as key challenges. Research networking organisations play a critical role in enabling scalable, network-centric earth and ocean observation.

How to cite: Ebrahimi, S., Loffredo, L., van den Hil, A., and Malhotra, R.:  Investigating subsea cable sensing for monitoring of marine life, detection of earthquakes and tsunamis with Research and Education network infrastructure, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19501, https://doi.org/10.5194/egusphere-egu26-19501, 2026.

EGU26-20683 | Orals | SM3.4

Distributed acoustic fibre sensing for large scientific infrastructures: ocean microseism at the European XFEL 

Celine Hadziioannou, Erik Genthe, Svea Kreutzer, Holger Schlarb, Markus Hoffmann, Oliver Gerberding, and Katharina-Sophie Isleif and the the WAVE initiative

The WAVE seismic network is a dense, multi-instrument monitoring system deployed on a scientific campus in Hamburg, Germany. It combines seismometers, geophones, and a 19 km distributed acoustic sensing fiber loop installed in existing telecommunication infrastructure. The network covers large-scale research facilities including the European X-ray Free-Electron Laser (EuXFEL) and particle accelerators at DESY. Its primary goal is to characterise natural and anthropogenic ground vibrations and to quantify how these signals couple into ultra-precise measurement infrastructures that are limited by environmental noise. Beyond local applications, WAVE serves as a testbed for fibre-optic sensing concepts relevant to fundamental physics, including seismic and strain monitoring for gravitational wave detection.

The EuXFEL is a femtosecond X-ray light source designed for ultrafast imaging and spectroscopy. Its performance depends critically on precise timing and synchronisation of the electron bunches along the linear accelerator. Measurements of bunch arrival times reveal significant noise contributions in the 0.05–0.5 Hz frequency band, with peak-to-peak timing jitter of up to 25 femtoseconds. Using distributed acoustic sensing data, we demonstrate that this jitter is largely explained by secondary ocean-generated microseism, which is identified as a significant limiting factor for stable, high-precision XFEL operation in the sub-Hz regime. 

To assess the potential for prediction and mitigation, we investigate whether ocean wave activity in the North Atlantic can be used to anticipate microseismic signals observed at the EuXFEL site. Output from the WAVEWATCH III ocean wave model is used to generate synthetic Rayleigh wave spectrograms with the WMSAN framework. These are compared to seismic observations at the EuXFEL injector. By subdividing the North Atlantic into source regions, we evaluate their relative contributions to the observed seismic wavefield. While absolute amplitude prediction remains challenging, the modelling reproduces key spectral characteristics and temporal variability.

Our results demonstrate that combining dense fibre-optic sensing with physics-based ocean wave modelling provides a framework to characterise microseismic noise and assess its limiting impact on high-precision experiments. This approach supports noise mitigation efforts at high-precision accelerator facilities and is directly relevant to future ground-based gravitational wave detectors.

How to cite: Hadziioannou, C., Genthe, E., Kreutzer, S., Schlarb, H., Hoffmann, M., Gerberding, O., and Isleif, K.-S. and the the WAVE initiative: Distributed acoustic fibre sensing for large scientific infrastructures: ocean microseism at the European XFEL, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20683, https://doi.org/10.5194/egusphere-egu26-20683, 2026.

EGU26-21683 | Posters on site | SM3.4

Leveraging Railway Fiber-Optic Networks with DAS: Multi-Scale Opportunities 

Pascal Edme, Daniel Bowden, Frederick Massin, Anne Obermann, sanket Bajad, John Clinton, and James Fern

Distributed Acoustic Sensing (DAS) enables the acquisition of seismic data with unrivalled spatio-temporal resolution over very large distances. Railway fiber-optic networks, originally deployed for telecommunications, offer cost-effective opportunities to monitor and characterize the subsurface at multiple scales. Here, we present a project conducted with the Swiss Federal Railways (SBB) involving the interrogation of dark fibers running along two perpendicular railway tracks, each approximately 40 km long. Data were acquired over three months using a dual-channel Sintela Onyx interrogator, with variable acquisition setups (spatial sampling, gauge length, and sampling frequency) tailored to different scientific objectives described below.

The primary objective was to assess the feasibility of using pre-existing telecommunications fibers for structural track-bed monitoring, specifically shallow subsurface Vs characterization through inversion of Rayleigh-wave dispersion curves (MASW). This requires high spatial sampling and short gauge length (3 m and 6 m, respectively) to capture short wavelengths. Several ambient noise interferometry strategies were tested, including stacking (1) all available time windows with various preprocessing schemes, (2) only time windows exhibiting strong directional wavefields, and (3) a coherent-source subsampling approach based on a Symmetric Variational Autoencoder to identify time windows contributing the most useful seismic energy. Unsurprisingly, trains constitute the most energetic and reliable seismic sources, from which dense Vs profiles can be derived, demonstrating the effectiveness of both the processing and inversion workflows.

Beyond shallow characterization, the experiment also yielded valuable data to complement dense nodal arrays deployed near Lavey-les-Bains, a site of significant geothermal interest and complex geological structure. The main objectives in this context are to (1) help characterizing the subsurface over the first kilometers, (2) investigate its relationship to geothermal circulation, (3) evaluate the joint use of dense nodal and DAS data for imaging, and (4) establish a high-quality, open-access dataset to support the development of next-generation passive imaging methodologies.

Finally, at an even larger scale, the experiment provided the opportunity to explore how DAS data can be leveraged within the operational Swiss Seismological Service (SED) network and to assess whether DAS can augment standard seismicity catalogues. Lower-resolution data (100 m spatial sampling, 200 Hz sampling frequency) were streamed and converted in real time into standard seismic formats (miniSEED and StationXML), demonstrating the feasibility of integrating DAS data into SeisComP for both automatic and manual processing.

We will present the dataset along with key results relevant to the three purposes outlined above.

We acknowledge Allianz Fahrbahn (grant agreement No. 100 072 202) for enabling this study.

How to cite: Edme, P., Bowden, D., Massin, F., Obermann, A., Bajad, S., Clinton, J., and Fern, J.: Leveraging Railway Fiber-Optic Networks with DAS: Multi-Scale Opportunities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21683, https://doi.org/10.5194/egusphere-egu26-21683, 2026.

EGU26-1250 | ECS | Orals | GI4.5

Advanced Volcanic Monitoring: AI Super-Resolution for Thermal Satellite Images 

Giovanni Salvatore Di Bella, Claudia Corradino, and Ciro Del Negro

Image Super-Resolution (SR) models are advanced image processing techniques designed to increase the spatial resolution of digital images by reconstructing fine details from low-resolution inputs while preserving essential characteristics of the original data. SR methods are particularly valuable when high spatial detail is needed but not directly available, enhancing the interpretability of degraded or coarse imagery.

In satellite thermal observations, SR is especially relevant. Thermal Infrared (TIR, 8–14 µm) images, used to measure surface thermal radiation, generally exhibit low spatial resolution and higher noise than optical imagery. These limitations hinder the identification and quantification of fine-scale thermal features, including localized hotspots, small eruptive vents, and narrow lava flows.

Here, we propose a super-resolution method for multispectral thermal images based on advanced artificial intelligence, implemented through a deep Residual Neural Network (ResNet) architecture. Trained on paired low- and high-resolution thermal datasets, the model learns the complex non-linear relationships required to recover high-frequency spatial information typically lost in coarse TIR imagery. Residual learning allows the network to focus on reconstructing missing fine-scale structures, improving training stability and enhancing subtle thermal gradients. The architecture mitigates vanishing-gradient issues and enables deeper networks capable of extraxùcting thermally meaningful features without amplifying noise.

The resulting model reconstructs fine thermal structures—such as narrow lava flows and localized hotspots—producing coherent and physically interpretable thermal maps. ResNet-based SR enables the integration of the broad coverage offered by low-resolution sensors with the detail provided by high-resolution platforms.

From a volcanic monitoring perspective, thermal SR improves the detection and tracking of eruptive features, providing more precise and timely information on volcanic activity. Overall, applying advanced SR techniques to satellite thermal imagery enhances active volcano surveillance and contributes to a more accurate understanding of volcanic thermal processes.

How to cite: Di Bella, G. S., Corradino, C., and Del Negro, C.: Advanced Volcanic Monitoring: AI Super-Resolution for Thermal Satellite Images, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1250, https://doi.org/10.5194/egusphere-egu26-1250, 2026.

EGU26-1526 | Orals | GI4.5

Optimization of DirecTES thermal infrared land surface temperature and emissivity separation algorithm for the upcoming TRISHNA mission 

Maxime Farin, Sébastien Marcq, Emilie Delogu, Didier Ramon, and Thierry Elias

The inversion of the radiative transfer equation to retrieve both the surface temperature (LST) and emissivity (LSE) values from top-of-atmosphere (TOA) radiances in the thermal infrared (TIR) domain (8-14 µm) is a not straightforward problem. Marcq et al. (2023) proposed the algorithm DirecTES to invert LST using a spectral library of emissivity of various materials, to be applied on several TIR channels.  The algorithm consists in inverting the radiative transfer equation for the LST, for each material of the library. A threshold criterion selects materials of the library for which the standard deviation of retrieved LST across different TIR channels is below 3K. The final LST and LSE are the median of the values retrieved for the selected materials. However, a constant threshold is problematic because sometimes no material in the library may match the criterion and thus the LST may not be retrieved on some pixels of a satellite image. Moreover, DirecTES’s original spectral library (SAIL179) is only composed of vegetation and arid surface materials and performs poorly on desertic surface pixels.

This study focuses on optimizing DirecTES in the TIR channels of the upcoming TRISHNA instrument conjointly developed by CNES (France) and ISRO (India). A new universal spectral library of emissivity that could be applied to any type of observed land surface of the globe is built with 150 emissivity spectra from the CAMEL database, categorized into four main classes (arid, desert, snow-covered or vegetated). In most cases, the category of the observed surface in a satellite image pixel is not known. We propose an optimization of DirecTES’s criterion that consists in selecting from the spectral library only the 10 materials with the lowest LST standard deviation between TIR channels. This new approach efficiently selects materials in the appropriate emissivity category on any surface, thus reducing the bias and RMS error on the retrieved LST and LSE. In addition, this new approach corrects the limitation of the original DirecTES criterion and can retrieve the LST and LSE on every pixel of the processed image.

The performances of the new DirecTES criterion and spectral library are evaluated, using TOA radiances simulated from the CAMEL emissivity database and the TIGR atmospheric database. LST is retrieved with a biais < 0.1K and a RMSE < 0.6K on vegetated surfaces and < 0.8K on arid and desert surfaces. LSE is retrieved with a RMSE < 0.02 for all TRISHNA TIR wavelengths. For desertic areas, performances are further improved when adding a few more emissivities from these specific regions to the spectral library used by DirecTES, while not affecting the performances on the other regions.

Finally, DirecTES is validated with match-up data of TOA radiances measured by ECOSTRESS and LST ground measurement at La Crau, France. For 53 match-ups dates of 2023, the LST is retrieved with a bias < 0.15K and RMSE < 0.9K.

How to cite: Farin, M., Marcq, S., Delogu, E., Ramon, D., and Elias, T.: Optimization of DirecTES thermal infrared land surface temperature and emissivity separation algorithm for the upcoming TRISHNA mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1526, https://doi.org/10.5194/egusphere-egu26-1526, 2026.

Ground-based hyperspectral longwave infrared (LWIR) images of 90 soil samples from the legacy soil spectral library of Israel were acquired with the Telops Hyper-Cam sensor. Mineral-related emissivity features were identified and used to create indicants and indices to determine the appearance and content of quartz, clay minerals, and carbonates in the soil in a semi-quantitative manner—from more to less abundant minerals. The resultant most abundant mineral(s) fit the results of the XRD analysis in most (90%) of the soil samples. The full mineralogy, including the relative amounts of the less abundant minerals, of most (75%) of the soil samples fit the XRD analysis results.

These hyperspectral LWIR images were resampled to the multispectral LWIR configurations of the airborne sensor Airborne Hyperspectral Scanner (AHS) and present and future spaceborne sensors—Land Surface Temperature Monitoring (LSTM), ECOSTRESS and Thermal Infra-Red Imaging Satellite for High-resolution Natural Resource Assessment (TRISHNA). The emissivity spectrum of each soil sample was calculated and then spectral indicants were created, for each spectral configuration, to determine the content of quartz, clay minerals and carbonates in each soil. The resulted mineral classification, in all spectral configurations, of the most abundant mineral(s) fit the XRD analysis results in most (90-80%) of the soil samples. However, identifying the less abundant minerals in each soil, and determining the mineralogy, from more to less abundant, using multispectral-based created indicants, was enabled only with the AHS configuration.

 

How to cite: Ben-Dor, E. and Notesko, G.: Spectral indicants to determine the most abundant mineral(s) in soil samples,using LWIR hyper- and multi- spectral configurations., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1662, https://doi.org/10.5194/egusphere-egu26-1662, 2026.

EGU26-3614 | Orals | GI4.5

Evaluation of Improved Hyperspectral Gas Detection Algorithms Using Hyper-Cam Airborne Nano Airborne Data 

Jean-Philippe Gagnon, Martin Larivière-Bastien, and Antoine Dumont

Evaluation of Improved Hyperspectral Gas Detection Algorithms Using Hyper-Cam Airborne Nano Airborne Data

Hyperspectral remote sensing enables the accurate characterization of gases from a distance, providing a safe and efficient means to identify gas releases for research, industrial monitoring, and threat assessment of unknown substances. Recent advances in airborne hyperspectral imaging systems—such as Telops’ Hyper-Cam Airborne Nano, a compact long-wave infrared (LWIR) hyperspectral imager—illustrate the growing capability to acquire spatially and spectrally resolved infrared measurements from aerial platforms. Telops hyperspectral systems have long been at the forefront of gas detection, identification, and quantification using thermal infrared imaging. However, improving the spectroscopic accuracy of hyperspectral imaging systems while maintaining spatial resolution remains a challenge, particularly when compared to the high spectral resolution of one-dimensional instruments. The work presented here showcases ongoing efforts to enhance hyperspectral gas analysis through the development of a new detection and identification (D&I) algorithm designed to improve multiple stages of the detection process.

 

D&I Algorithm Improvements

The updated algorithm builds on the original GLRT (Generalized Likelihood Ratio Test) which is good for detecting spectral anomaly that correlates with a given spectrum, but which is often non-specific. Within the new algorithm, the GLRT-detected pixels are then grouped together according to their spatial connection to get a list of plumes to investigate. The spectral radiance of the whole datacube is then separated in clusters of similar pixels. Using principal component analysis (PCA), the background behind the plume of interest is estimated. Using the background, the plume spectral transmittance is estimated. The spectral transmittance is then compared to the theoretical signature to get a similarity value (correlation) for each investigated plume. A threshold is applied to eliminate all plumes which are considered as false alarm. Throughout the work, it was mandatory to have fewer false alarms compared to the old algorithm, maintain real-time detection and identification performances and good performances for ground based and airborne operations.

Results

The dataset used to evaluate the new algorithm consists of several controlled gas release experiments conducted under varied conditions for both ground-based and airborne configurations. A portion of the results presented here is derived from a recent airborne data collection campaign performed using the Hyper-Cam Airborne Nano hyperspectral imaging system. Algorithm performance was quantified using Receiver Operating Characteristic (ROC) curves (true positive rate versus false positive rate) to compare the new algorithm against the previous implementation. The selected performance metric—the integral of the ROC curve between 0 and 0.1 false positive rate—increased from 0.0279 for the original algorithm to 0.0623 for the updated version, representing more than a twofold improvement (Figure 2). These results demonstrate a significant reduction in false alarms for common objects (e.g., vehicle windshields, clothing, quartz), unrelated gaseous signatures, and motion-induced artefacts, while maintaining robust detection performance.

How to cite: Gagnon, J.-P., Larivière-Bastien, M., and Dumont, A.: Evaluation of Improved Hyperspectral Gas Detection Algorithms Using Hyper-Cam Airborne Nano Airborne Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3614, https://doi.org/10.5194/egusphere-egu26-3614, 2026.

A long, high-quality, and temporally continuous high spatiotemporal resolution air temperature (Ta) dataset plays a crucial role across various domains, particularly in areas such as human health, disease prediction and control, and energy utilization, where extreme temperatures (daily maximum and minimum temperatures) hold significant value. However, due to the instability of extreme temperatures influenced by various factors like topography, altitude, climate, and underlying surfaces, coupled with sparse meteorological station coverage, traditional methods struggle to accurately capture and produce high-quality, temporally continuous temperature dataset products. In this study, the four-dimensional spatiotemporal deep forest (4D-STDF) model was utilized, based on daily meteorological station temperature data from 2003 to 2022, along with seamless daily LST, meteorological, radiational, land use, topographic and population data encompassing 12 parameter factors and 6 spatiotemporal factors, three high-quality daily Ta datasets were constructed and generated. These datasets cover mainland China, featuring high spatial resolution (1km), long temporal sequences (2003-2022), and increased accuracy. The datasets include maximum (Tmax), minimum (Tmin), and mean (Tmean) temperatures from January 1, 2003, to December 31, 2022, as well as monthly and yearly synthesized Tmax, Tmin, and Tmean values, presented in GeoTIFF format with WGS84 projection, and the data unit is in 0.1 degrees Celsius (°C). The overall RMSE values are 1.49°C, 1.53°C, and 1.18°C for daily estimates, 1.38°C, 1.65°C, and 0.52°C for monthly, and 1.28°C, 1.83°C, and 0.41°C for annual, respectively. These datasets reasonably capture the spatial and temporal heterogeneity of Ta and effectively capture the intensity of heatwaves and cold spells. These new datasets are of significant value for studying extreme climates and contribute to assessing their impact on human health, infrastructure, and energy demands.

How to cite: Luan, Q.: Estimation of all-sky daily air temperature with high accuracy from multi-sourced data in China from 2003 to 2022, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4371, https://doi.org/10.5194/egusphere-egu26-4371, 2026.

Pre-eruptive, long-term, large-scale thermal anomalies detectable in 1 km resolution MODIS Thermal Infrared (TIR) radiance data have been consistently observed at long-dormant volcanoes years before eruptions. However, the physical mechanisms driving these signals remain unresolved. This study addresses a critical question: is the large-scale thermal anomaly primarily governed by localized high-temperature conduit heating or by spatially distributed, low-intensity heat release from diffuse magmatic degassing along volcanic flanks? Resolving this mechanism is vital for interpreting TIR data and for understanding heat and volatile transport during volcanic unrest.

We investigate this question at Augustine Volcano during its 2006 eruption, where summit conduit warming preceded the large-scale thermal anomaly by approximately three months. To explain this temporal offset, we adopt a conceptual model following Zhan et al. (2022), based on magma ascent followed by conduit sealing. We simulate surface thermal evolution under two scenarios: (1) an area-integrated signal including both the conduit and flanks, and (2) a conduit-excluded signal (near-vent area, ~150 m radius removed) dominated by flank degassing. The simulations show that including the conduit produces rapid warming synchronous with summit heating, whereas conduit-excluded simulations yield a delayed warming that reproduces both the timing and magnitude of the observed large-scale anomalies.

The strong agreement between conduit-excluded simulations and satellite observations provides robust evidence that the pre-eruptive thermal anomaly at Augustine was predominantly controlled by diffuse flank degassing rather than conduit heating. More broadly, our study establishes a physically-based framework for interpreting satellite thermal anomalies as indicators of evolving degassing pathways and subsurface permeability changes during prolonged volcanic unrest. This significantly enhances the utility of TIR monitoring for understanding volcanic heat transport processes and the state of unrest. Furthermore, we plan to apply this framework to a wide range of volcanoes to evaluate the generality of these findings.

How to cite: Chenyan, W. and Zhan, Y.: Diffuse Flank Degassing as the Dominant Source of the Large-Scale Thermal Anomaly Preceding the 2006 Augustine Eruption, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8833, https://doi.org/10.5194/egusphere-egu26-8833, 2026.

EGU26-10084 | Posters on site | GI4.5

Revealing heat patterns of lava flows: a spatial data analysis approach using UAV thermography 

Héctor de los Rios-Díaz, David Afonso-Falcón, Víctor Ortega-Ramos, Aarón Álvarez-Hernández, Luis González-de-Vallejo, Nemesio M. Pérez, and Pedro A Hernández

The 2021 Tajogaite eruption on La Palma (Canary Islands, Spain) generated extensive lava flows that still exhibit measurable residual surface heat several years after the eruption. Understanding the spatial distribution and persistence of this heat is essential for characterizing post-eruptive cooling processes and for supporting reconstruction activities in affected areas. 

An integrated geospatial workflow was implemented to combine high-resolution UAV-based thermal imagery with lava-thickness models across two sectors affected by the eruption: LPAgricultura (surveyed in February 2024) and LPUrban (surveyed in June 2025). Drone-based radiometric infrared imagery was processed to produce georeferenced thermal mosaics, with emissivity correction (ε = 0.95), and resampled to match the spatial resolution of the corresponding lava-thickness datasets. All data were aligned within a common spatial reference system (REGCAN95 / UTM zone 28N) to ensure pixel-level correspondence. 

Thermal anomalies were defined as surface temperatures equal to or exceeding 30 °C. Lava-thickness values were extracted separately for thermally anomalous and non-anomalous areas, enabling a consistent spatial comparison between the two conditions. Statistical analyses were conducted independently for each sector to evaluate the relationship between residual heat and flow thickness. 

Results reveal a clear,statistically significant association between elevated surface temperatures and thicker lava deposits across the Tajogaite lava field. In the LPUrban sector, characterized by thicker lava accumulations (mean thickness = 21.5 m; maximum = 57.1 m), thermally anomalous areas have a mean thickness of 31.3 m, compared with 21.3 m in non-anomalous zones (p < 0.001). In contrast, the LPAgricultura sector, dominated by thinner flows (mean thickness = 9.2 m; maximum = 51.5 m), shows mean thickness values of 20.6 m in anomalous areas versus 10.0 m elsewhere (p < 0.001). These patterns indicate that residual heat is preferentially concentrated within the thickest portions of the lava flows, where cooling is constrained by reduced surface-to-volume ratios and enhanced thermal insulation. The adoption of relative thickness thresholds (≥ 20 m in urban areas and ≥ 10 m in agricultural areas) captures approximately 95% of the total surface area of detected thermal anomalies, ensuring consistent sensitivity across both sectors.  

The combined use of UAV thermography and lava-thickness models enables a robust characterization of post-eruptive thermal persistence, with direct implications for the assesing lava-flow cooling behavior in complex volcanic terrains. 

How to cite: de los Rios-Díaz, H., Afonso-Falcón, D., Ortega-Ramos, V., Álvarez-Hernández, A., González-de-Vallejo, L., Pérez, N. M., and Hernández, P. A.: Revealing heat patterns of lava flows: a spatial data analysis approach using UAV thermography, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10084, https://doi.org/10.5194/egusphere-egu26-10084, 2026.

EGU26-10190 | Posters on site | GI4.5

Post-eruptive thermal evolution of the Tajogaite volcano and its relationship with volcano-structural settling 

David Afonso-Falcón, Héctor de los Ríos-Díaz, Victor Ortega-Ramos, Óscar Rodríguez-Rodríguez, Nemesio M.Pérez-Rodríguez, Luca DÁuria, and Pedro Antonio-Hernández

The 2021 eruption of the Tajogaite volcano (La Palma, Canary Islands) produced a new volcanic cone whose post-eruptive thermal evolution and structural adjustment remain active processes of considerable scientific interest.  Characterising how surface temperature patterns evolve over time and how they relate to morphological changes is essential for understanding the stabilization phase of newly formed volcanic edifices. 

This study aims to provide a preliminary assessment of the post-eruptive thermal evolution of the Tajogaite cone and to explore its potential relationship with volcano-structural settling. 

The analysis integrates multi-temporal UAV-derived thermal imagery and digital elevation models (DEMs). Four thermal UAV surveys acquired at different post-eruptive stages were processed and homogenized in terms of spatial reference, resolution, and alignment to ensure temporal comparability. Two representative periods were selected to analisechanges in surface temperature distribution, while DEMs from two different dates were used to assess morphological variations. Data pre-processing included reprojection, resampling, and quality control procedures, whose reliability was evaluated through statistical comparisons and profile-based analyses. Thermal difference maps and elevation change analyses were subsequently generated. 

The results reveal spatially coherent thermal patterns and detectable differences between the analysed periods, consistent with an overall cooling tendency and localized morphological adjustments. These patterns suggest a spatial relationship between surface temperature evolution and structural changes of the volcanic cone, although the magnitude and significance of these relationships require further investigation. 

Although preliminary, the results indicate that the combined use of UAV-based thermal data and DEMs is a suitable approach for monitoring post-eruptive volcanic cones. The proposed workflow provides a reproducible methodological framework that may support future, more detailed analyses of cooling dynamics and volcano-structural evolution in newly formed volcanic landforms. 

How to cite: Afonso-Falcón, D., de los Ríos-Díaz, H., Ortega-Ramos, V., Rodríguez-Rodríguez, Ó., M.Pérez-Rodríguez, N., DÁuria, L., and Antonio-Hernández, P.: Post-eruptive thermal evolution of the Tajogaite volcano and its relationship with volcano-structural settling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10190, https://doi.org/10.5194/egusphere-egu26-10190, 2026.

EGU26-12526 | ECS | Orals | GI4.5

Characterization of Urban Surface Materials using Airborne Imaging FTIR Spectroscopy: First Results from a Campaign in Dessau, Germany 

Josef William Palmer, Bastian Sander, Milena Marković, and Marion Pause

Imaging Fourier-Transform Infrared (FTIR) spectroscopy in the long-wave infrared (LWIR) domain (7–14 µm) offers unique capabilities for the identification and mapping of surface materials based on their distinct spectral emissivity signatures. While laboratory applications are well-established, airborne deployment for complex urban environments remains a developing field. This study presents initial results from a recent test campaign conducted on the 20th of May 2025 in Dessau, Germany by utilizing the Telops Hyper-Cam Airborne Mini. The objective of this research was to evaluate the sensor's capability to detect and discriminate common urban surface materials such as concrete, asphalt, roofing tiles, and potentially polymers and metals under real-world flight conditions. The hyperspectral data cubes were acquired over an industrial urban area at an altitude of around 800 meters above ground resulting in a resolution of 60 cm per pixel with a spectral resolution of 6.5 wavenumbers. The airborne measurements were validated through comparison with a laboratory-based spectral reference library acquired under controlled conditions. The comparison with laboratory spectra provides critical insights into the reliability of airborne FTIR data. In particular, we utilized a spectral library developed by King’s College London as a reference standard, consisting of representative material samples collected from the London area. We performed a comparative analysis between the atmospherically corrected airborne emissivity spectra (processed by FLAASH-IR) and the laboratory emissivity reference signatures. The results demonstrate a strong correlation between the airborne data and the laboratory measurements. Specifically, the system showed high proficiency in distinguishing between silicate-based materials and metal due to their characteristic absorption and emissivity features in the LWIR region. However, challenges remain in classifying asphalt, solar panels, and roofing materials due to surface conditions and low spectral contrast as well as the problem of spectral mixing. This study highlights the potential of the Telops Hyper-Cam Airborne Mini for hyperspectral urban material mapping and addresses challenges that need to be solved in the future. Our findings contribute to a better understanding of urban surface heterogeneity and support the planning of future airborne campaigns for urban planning and environmental monitoring applications.

This research is funded by the German Research Foundation (DFG, grant number: 514067990).

How to cite: Palmer, J. W., Sander, B., Marković, M., and Pause, M.: Characterization of Urban Surface Materials using Airborne Imaging FTIR Spectroscopy: First Results from a Campaign in Dessau, Germany, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12526, https://doi.org/10.5194/egusphere-egu26-12526, 2026.

EGU26-13110 | Orals | GI4.5

CEOS Analysis Ready Data Surface Temperature Product Family Specification V6.0 

Siri Jodha Khalsa, Harvey Jones, Matthew Steventon, Peter Strobl, Anastasia Sarelli, and Josephine Wong

The Committee on Earth Observation Satellites (CEOS) produces and maintains a series of Analysis Ready Data (CEOS-ARD) Product Family Specifications (PFS) across Earth observation technologies. Each PFS provides a mandated list of specifications for pre-processing, metadata, and documentation, providing value for interoperability, benchmarking, procurement, and user confidence.

This submission presents an overview and update on the CEOS-ARD Surface Temperature (ST) PFS Version 6.0, which recognises and accommodates the evolving user base, technology, and applications of space-based infrared data from public and commercial sector missions. The ST PFS applies to designers and deployers of missions operating in the thermal infrared (TIR and MWIR) and microwave wavelengths at all scales.

New metadata requirements are being introduced to support the varying types of surface temperature products: land surface temperature, surface brightness temperature, and water surface temperature. The PFS also features updates in line with the Future CEOS-ARD Strategy, with modifications to requirements on data quality, radiometric stability, and other general metadata while also providing better support for higher level applications and harmonisation between CEOS-ARD PFS. The CEOS-ARD Oversight Group invites feedback, contribution, and early adoption. 

More information on CEOS-ARD can be found at ceos.org/ard.

How to cite: Khalsa, S. J., Jones, H., Steventon, M., Strobl, P., Sarelli, A., and Wong, J.: CEOS Analysis Ready Data Surface Temperature Product Family Specification V6.0, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13110, https://doi.org/10.5194/egusphere-egu26-13110, 2026.

EGU26-13700 | Posters on site | GI4.5

Multiplatform TIR remote sensing for monitoring and surveillance of the Campi Flegrei caldera. 

Enrica Marotta, Andrea Barone, Rosario Peluso, Gala Avvisati, Francesco Mercogliano, Andrea Vitale, Malvina Silvestri, Eliana Bellucci Sessa, Pasquale Belviso, Maria Fabrizia Buongiorno, and Pietro Tizzani

Thermal infrared (TIR) remote sensing is an increasingly used technique for studying various natural and anthropogenic processes by evaluating the thermal state of the Earth’s surface. Technological advancements have supported the development of thermal cameras for ground-based, airborne, and satellite platforms. Additionally, Unmanned Aerial Systems (UAS) are increasingly regarded as versatile platforms due to their flexible observation scales.

In a volcanic framework, TIR remote sensing enables the study of ground temperature and the identification of thermal anomalies caused by hot fluid discharge (e.g., gas and lava) or surface heating due to fluid migration in the subsoil during unrest phases, which modify the pressure and temperature conditions of the crust. TIR remote sensing is therefore an essential tool for monitoring and surveillance of active volcanoes, although the spatial coverage and resolution of planned surveys can sometimes be inadequate for emergency management. Indeed, ground-based measurements do not guarantee extensive spatial coverage, while satellite data lack flexibility regarding spatial and temporal resolutions. Finally, airborne measurements are challenging to organize operationally during emergencies and are inherently risky. In this scenario, UAS platforms represent a reasonable trade-off in terms of spatial coverage, resolution, and logistics.

Here, we present a case study of multiplatform (satellite and UAS) TIR remote sensing as part of the monitoring activities at the Campi Flegrei caldera by INGV – OV. This active volcanic system is characterized by complex interactions between magmatic and hydrothermal reservoirs, causing frequent unrest with ground deformation, seismicity, gas emissions, and surface temperature anomalies. Among the latter, we focus on the most significant anomalies located near the Solfatara – Pisciarelli hydrothermal system.

Satellite measurements consist of nighttime images acquired by the Landsat-8 and Landsat-9 satellites from May 2018 to August 2025, with a 100 m spatial resolution, processed to retrieve an approximately monthly distribution of Land Surface Temperature (LST). Conversely, UAS data consist of images acquired monthly by INGV – OV with a 10 cm spatial resolution at flight altitudes ranging from 45 to 70 m. For logistical reasons, the Pisciarelli dataset spans from September 2019 to May 2025, while images of Solfatara were only acquired during the first halves of 2024 and 2025.

The results show that satellite data can detect a single anomaly at the Solfatara – Pisciarelli hydrothermal system without revealing significant temporal variations in temperature. On the other hand, UAS data identify multiple anomalies for both the Solfatara and Pisciarelli sites, highlighting surface heating in Pisciarelli starting around September 2021. This trend is consistent with analyzed seismicity and ground deformation datasets.

This study demonstrates the role of multiplatform TIR data integration in improving monitoring and surveillance activities at active volcanoes.

How to cite: Marotta, E., Barone, A., Peluso, R., Avvisati, G., Mercogliano, F., Vitale, A., Silvestri, M., Sessa, E. B., Belviso, P., Buongiorno, M. F., and Tizzani, P.: Multiplatform TIR remote sensing for monitoring and surveillance of the Campi Flegrei caldera., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13700, https://doi.org/10.5194/egusphere-egu26-13700, 2026.

EGU26-14067 | ECS | Posters on site | GI4.5

UAV-Based Modeling of Land Surface Temperature Using Machine Learning Methods 

Oleksandr Hordiienko and Jakub Langhammer

Land Surface Temperature (LST) is an important climate variable that helps us understand surface heat processes and environmental change. This study focuses on identifying scales at which LST can be reliably modeled using high-resolution RGB and near-infrared (NIR) data as the main input predictors. The approach is based on the well-known negative correlation between the Normalized Difference Vegetation Index (NDVI) and  LST, while vegetation indices represent only one component of the surface energy balance. The study frames LST modeling as a data-driven emulation problem, where surface properties derived from RGB–NIR imagery are combined with concurrent atmospheric and environmental conditions. Several machine learning methods are tested, including Random Forest, XGBoost, LightGBM, and Convolutional Neural Networks, to build an LST emulation framework that links spectral surface information with observed thermal patterns under varying environmental conditions.

The study area is located in the Šumava Mountains in the Czech Republic, a mountain peatland with high ecological value and sensitivity to climate change. Data was collected using a UAV platform between 2025 and 2026, equipped with two sensors: an RGB–NIR camera for surface characterization and a thermal camera used as reference data for surface temperature. These paired multispectral and thermal UAV data form the training basis for the machine-learning models. To ensure the reliability of the models, UAV-derived LST was validated using multiple independent data sources, including in-situ Thermal Infrared (TIR) measurements, near-ground air temperature and humidity monitoring, or air temperature measurements from nearby weather stations.

In addition to spectral variables, the models include several environmental factors that influence surface temperature, such as solar angle, air humidity, soil moisture, wind speed, and canopy height, which act as physical controls on the modeled LST.  A key goal of the study is to test the potential of transfer learning by training the models on data from the Šumava Mountains and evaluating their performance when applied to data from a different season, thereby assessing the temporal robustness of the emulation approach under changing atmospheric and surface conditions.

How to cite: Hordiienko, O. and Langhammer, J.: UAV-Based Modeling of Land Surface Temperature Using Machine Learning Methods, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14067, https://doi.org/10.5194/egusphere-egu26-14067, 2026.

The use of high spatial resolution orbital thermal infrared (TIR) data for certain geoscience applications has been possible for the past four decades. Satellites having one or two TIR spectral bands were able to detect the spatial patterns and temporal baselines of surface temperature; however, they do not provide any information on emissivity variation (essential for mapping critical minerals), and less accurate temperatures than multispectral TIR systems. In 2000, ASTER (the first multispectral TIR sensor with sub 100 m spatial resolution) was launched and has acquired data for over 25 years but will be decommissioned in 2026. A similar instrument (ECOSTRESS) was launched to the International Space Station (ISS) in 2018 and is still functioning, but it will be retired in 2030 with the ISS leaving a gap in US multispectral TIR capability. Multispectral TIR data expanded what was possible in the geosciences, providing compositional information such as surface mineralogy, thermal inertia, and particulate mapping, together with more accurate and refined uses of surface temperatures. Several countries/space agencies are planning high spatial, high temporal resolution multispectral TIR missions in the near future that will provide continuity and greatly expand possible applications with much higher repeat times. One of these, the Surface Biology and Geology (SBG-TIR) mission would provide MIR (3–5 μm) and TIR (8–12 μm) image data at ~ 60 m spatial resolution every 1-3 days. SBG-TIR is a joint-endeavor between NASA and ASI in Italy with planned geoscience data products such as surface mineralogy and volcanic activity, whereas the other planned missions do not have this geological focus. The TIR spectral resolution was increased to six bands for SBG-TIR, which vastly improves the capability of discriminating feldspar and clay mineralogy mapping as well as aerosol detection in sulfur dioxide rich plumes. The global mapping of the major rock-forming minerals and their weight percent silica together with the detection of subtle thermal and compositional changes at volcanoes will be possible for the first time with SBG-TIR. As part of the mission development, our work examined prior ASTER and airborne MASTER TIR data to test both the mineral mapping and precursory thermal volcanic eruption signal detection possible with SBG-TIR. ASTER provides the long time series to quantify low-level anomalies and small eruption plumes over long periods, whereas the airborne MASTER provides the spectral resolution necessary to identify minerals. The findings of the surface mineralogy and volcanic activity algorithm development will be presented and compared to those from the other planned TIR missions with lower spectral resolutions. Critically however, the SBG-TIR mission’s future is now uncertain due to recent budgetary reductions by the United States federal government. While the other European multispectral TIR mission move ahead, NASA is in danger of permanently losing its advantage in this technology space. This looming high resolution, multispectral TIR gap will reduce science outcomes and render others such as mineral mapping impossible.

How to cite: Ramsey, M., Hook, S., and Thompson, J.: Advancing the geosciences with thermal infrared orbital data: Future possibilities or a looming data gap? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14391, https://doi.org/10.5194/egusphere-egu26-14391, 2026.

EGU26-14953 | Orals | GI4.5

Monitoring precursory volcanic activity: Applying convolutional neural networks to the decades-long ASTER archive 

Claudia Corradino, Sophie Pailot-Bonnétat, Michael S. Ramsey, James O. Thompson, and Evan Collins

The next generation of thermal infrared (TIR) sensors will provide higher spatial and temporal resolution data than currently available. These include the ISRO-CNES’s Thermal infraRed Imaging Satellite for High-resolution Natural Resource Assessment (TRISHNA), ESA’s Land Surface Temperature Monitoring (LSTM), and NASA-ASI’s Surface Biology and Geology (SBG) missions. The near-daily coverage at ~60m spatial resolution will be invaluable for volcano monitoring but introduces new challenges. The large and complex data volumes from these missions require new advanced analytical approaches for effective detection of volcanic unrest. The 25-year archive of 90 m spatial resolution TIR data from the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) has accurately detected both large surface temperature variations during eruptive activity and subtle anomalies (1-2K) associated with degassing and precursory summit activity. Preliminary studies on eruption forecasting potential used ASTER data to constrain models of magmatic and geothermal processes, both crucial for improving hazard mitigation. A machine learning (ML) version of the Automated Spatiotemporal Thermal Anomaly Detection (ASTAD) algorithm, a CNN-based model specifically designed for ASTER data, achieved improved detection rates. CNN models are well suited for extracting spatial and thermal features as well as identifying subtle anomalies. The combination of ASTER’s spatial resolution and ASTAD-ML’s pattern recognition capabilities allows us to retrospectively test the approach globally in preparation for future missions. Here, we show the capability of ASTAD-ML by designing a global cloud-based AI platform populated with ASTER data. We applied the ASTAD-ML model to 100 representative volcanoes spanning a wide range of thermal, morphological, and volcanological activity types. The model includes both day and night data, as well as scenes typically discarded due to cloud cover or partial data loss/stripping. We evaluated both pixel-based and event-based performance, achieving BF1 and F1 high scores of 0.80 and 0.89, respectively. The ASTAD-ML model's pattern recognition capabilities both expanded the usable dataset and improved the accuracy of automatic early volcanic unrest detection. The methodology is highly adaptive, and further testing is ongoing in preparation for these future high spatial resolution TIR sensors, enabling significantly improved monitoring of global volcanic activity.

How to cite: Corradino, C., Pailot-Bonnétat, S., Ramsey, M. S., Thompson, J. O., and Collins, E.: Monitoring precursory volcanic activity: Applying convolutional neural networks to the decades-long ASTER archive, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14953, https://doi.org/10.5194/egusphere-egu26-14953, 2026.

EGU26-14996 | ECS | Orals | GI4.5

From Anomaly to Detectability: Roof Thickness Threshold for Remote Detection of Lava Tubes Using Thermal Infrared Datasets 

Jelis Sostre-Cortes, Frances Rivera-Hernandez, and Benjamin McKeeby

Lava tubes are key targets for planetary exploration due to their potential to preserve biosignatures and could serve as human habitats on the Moon. These caves form when lava flows solidify, leaving behind a tube-like void once the lava drains. Their stability is determined mainly by the thickness of the roof, a parameter that is challenging to estimate using current remote sensing methods, as visible imagery alone cannot discern the physical properties of the subsurface. Accurate characterization of roof thickness is crucial for future exploration efforts, as stable roofs are more likely to preserve potential biosignatures within the cave interior and provide safer environments for human exploration. Remote sensing is currently the primary method for studying lava tubes on other planetary bodies and in remote regions of Earth. Previous work has identified potential subsurface voids on the Moon and Mars using thermal infrared (TIR) imaging by analyzing the area's thermal inertia and temperature differences between lava tubes and surrounding terrain. Thermal inertia is an intrinsic material property that determines the material's resistance to changes in temperature and is affected by subsurface voids, which disrupt heat transfer. This study aims to constrain the maximum roof thickness that a lava tube can have to be detected with TIR remote sensing data, which can help estimate the roof thickness of lava tubes on Earth and other planetary bodies.

We present field, remote sensing, and numerical results of the thermophysical properties of lava tubes on Earth at two sites: Pisgah Crater, California, and Tabernacle Hill, Utah, with a total of 38 skylights and lava tube entrances surveyed. Satellite TIR images were acquired and compared with in-situ drone-based TIR images, both of which were used to calculate the thermal inertia of the area. To validate these observations, we utilized numerical heat transfer models to simulate thermal diffusion through basaltic roofs of varying thicknesses. The known lava tube locations were mapped, and their thermal inertia value was averaged to calculate the thermal inertia difference from the rest of the void-free terrain. These values were compared with in-situ measurements of roof thickness at each cave entrance.

Our study reveals a distinct decrease in the thermal difference from the background with increasing roof thickness, suggesting that thicker roofs behave more like the surrounding terrain. The observed data suggest that a roof thickness of at most 2 meters is required for potential detection in an Earth environment. This research helps establish a critical detection threshold, where TIR anomalies may be diagnostic of thin, potentially unstable roofs, while roofs thicker than 2 meters are likely stable but thermally indistinguishable from the background. Thermal anomalies are more distinct than visible data alone for identifying skylights in rough terrains, but larger and more stable roofs may be more challenging to detect than smaller roofs. This research reinforces the utility of TIR in identifying skylights in rough terrains. It establishes an essential constraint for the detectability and stability of lava tubes, providing a valuable framework for planetary remote sensing and future mission planning.

How to cite: Sostre-Cortes, J., Rivera-Hernandez, F., and McKeeby, B.: From Anomaly to Detectability: Roof Thickness Threshold for Remote Detection of Lava Tubes Using Thermal Infrared Datasets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14996, https://doi.org/10.5194/egusphere-egu26-14996, 2026.

Drought-induced stress of crops increasingly threatens agricultural yields and consequently food production security, which becomes even more challenging due to growing climatic instability. Consequently, the early detection of water-stress-related responses in crops is important to administer precise irrigation as well as for identifying varieties resilient to drought.

While multi- and hyperspectral remote sensing in the visible, near-, and short-wave infrared (VNIR/SWIR, 0.4–2.5 µm) is an established and robust tool for spatially assessing and monitoring vegetation vitality, less focus has been given to high-resolution spectral data covering the long-wave infrared (LWIR) so far. However, advancements in airborne sensors close this gap and allow for capturing detailed spectral information of vegetation components that are sensitive to water stress and show their fundamental vibrational features in the LWIR. Against this background, this case study evaluates the potential of airborne hyperspectral LWIR emissivity and temperature data to differentiate crop species and varieties.

The experimental setup is located at the Strenzfeld agricultural test site close to Bernburg, Central Germany, and comprises 32 plots, each approximately 67 x 9 m. The study includes three crop species (peas, winter wheat, and summer barley) with two varieties each, planted in four replicates, alongside eight bare soil plots. Hyperspectral LWIR data (7.4–11.8 µm, spectral resolution 6 cm-1, spatial resolution 0.77 x 0.77 m) were recorded on 6 May 2025 using a Telops Hyper-Cam Airborne Mini. Data preprocessing, including geometric corrections and data cube mosaicking, was conducted using Reveal Airborne Mapper, while temperature-emissivity separation was employed via Reveal FLAASH-IR. Additionally, UAV-based broadband thermal data and RGB orthomosaics were acquired with DJI Zenmuse XT2 and DJI Zenmuse H20T sensors to coincide with the aircraft overpass.

Emissivity spectra and temperature data were analysed at the plot-level to identify crop-specific spectral features and assess inter- and intra-class variations. Principal Component Analysis (PCA) was used to explore clustering within the spectral data. To account for differences in vegetation cover and the background soil signal, (partial) unmixing approaches exploiting vegetation and bare soil emissivity spectra were used as well as spectral indices. Furthermore, an inter-comparison of the temperature values derived from the Hyper-Cam Airborne Mini and the DJI Zenmuse XT2 was performed.

The findings of this case study contribute to a better understanding of LWIR emissivity signatures of different crops and their variability. Initial results show that in addition to crop-specific traits, vegetation cover and thus the soil signal distinctively impact the observed emissivity and temperature values. This highlights the importance of selecting optimal phenological windows for data acquisition. A planned follow-up study will incorporate multi-temporal airborne LWIR data acquisitions and controlled irrigation experiments in order to identify crop varieties with increased drought-resilience.

This research is funded by the German Research Foundation (DFG, grant number: 514067990) and by the Federal Ministry of Agriculture, Food and Regional Identity (BMLEH, grant number: 28DE205A21).

How to cite: Denk, M., Sander, B., and Knauer, U.: Analysis of crop species and varieties using airborne long-wave infrared hyperspectral imaging: a case study at Bernburg-Strenzfeld, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18259, https://doi.org/10.5194/egusphere-egu26-18259, 2026.

EGU26-18480 | Posters on site | GI4.5

The Instrument Simulator for Infrared Sounder onboard Chinese SI-Tracable Satellite 

Lu Lee, Lei Ding, and Mingjian Gu

In order to utilize satellite observations to address the climate change concerns, a concept of benchmark measurement is defined, and finally lead to the SI-Traceable Satellites (SITSat) missions. Traceability refers to the ability to track a measurement to a known standard unit (such as the Système Internationale (SI) standards) within a given measurement uncertainty. The SI-traceable observations can better withstand measurement-data gaps, and reduce uncertainties in long-term instrument calibration drifts while in orbit. Besides, The SITSat can serve as a space metrology lab to calibrate other space instruments and convert them into a climate benchmarking system with excellent global coverage. Now, there are several SITSat missions are under development by some space agencies, including the TRUTHS developed in ESA, and the CLARREO developed in NASA. In 2014, China Ministry of Science and Technology initiated and funded the Chinese Spaced-based Radiometric Benchmark (CSRB) project, with the ultimate goal of launching a flight unit of SITSat named LIBRA.

As a part of the LIBRA mission, an infrared sounder (LIBRA-IRS) based on a Michelson interferometer is designed to have a spectral range from 600-2700 cm-1, with a spectral sampling of 0.5 cm-1. To maintain the SI traceability of IR radiance, a high emissivity blackbody source is used as the onboard absolute calibration source, which uses multiple phase-change cells to provide an in-situ standard with absolute temperature accuracy.

In the other hand, achieving ultra-high accuracy of 0.1 K (k=3) also depends on a well-designed instrument (IRS) and an accurate absolute calibration model. In order to identify and evaluate the uncertainty contributions in calibrated radiance, and thereby improve the traditional calibration approach, an end-to-end instrument simulator is developed in conjunction with IRS instrument development and testing.

The simulator is a computer software written in MATLAB, and can be regarded as a numerical abstraction of the physical sounder. It takes atmospheric or calibration scene radiance as well as instrument parameters as inputs, then converts them into interferograms through Fourier transformation and adds errors and noise. Finally, it generates sampled interferograms through an analog-to-digital converter (ADC). The atmospheric radiance is calculated by the Line-By-Line Radiative Transfer Model (LBLRTM) with a spectral sampling less than 0.01 cm-1. As for the instrument model, it includes all FTS relevant optical, mechanical, electronic and thermal physics such as: optical transmittance, interferometer modulation, moving mirror speed fluctuations and time-dependent tilt, polarization of optics, background thermal flux, self-apodization due to the extension of field of view, optical and electronics noise, detector spectral responsivity and response non-linearity, sampling laser wavelength, electronic signal chain and ADC quantization, etc. Subsequently, the simulated interferogram data of atmospheric and calibration scenes are input into the radiometric calibration model to produce the calibrated radiance. This simulator is helpful for understanding the instrument, analyzing the system performance, improving the instrument design through end-to-end error analysis, and providing proxy data for calibration algorithms and software development.

How to cite: Lee, L., Ding, L., and Gu, M.: The Instrument Simulator for Infrared Sounder onboard Chinese SI-Tracable Satellite, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18480, https://doi.org/10.5194/egusphere-egu26-18480, 2026.

EGU26-18886 | ECS | Orals | GI4.5

The effect of thermal image quality on the estimation of Crop Evapotranspiration 

Shahla Yadollahi and Bernard Tychon

Understanding the surface energy balance is essential for studying land-atmosphere interactions and their impact on weather, climate, and hydrology. Accurate estimation of sensible and latent heat fluxes is critical for applications like hydrological modelling and climate studies, but traditional methods like eddy covariance are limited in spatial coverage. Remote sensing technologies, particularly models like the Two-Source Energy Balance (TSEB), address these limitations by partitioning energy fluxes between soil and vegetation using spatially distributed observations such as surface temperature and vegetation indices. Advances in TSEB include refined resistance networks for modelling soil-canopy interactions and improved disaggregation of surface temperatures into soil and canopy components, with iterative algorithms enhancing flux partitioning. Challenges remain in accounting for vegetation clumping and accurate modelling in water-limited ecosystems. In this study, the potential of three thermal data providers, Ecostress and Landsat from NASA and Sentinel-3 from ESA, in estimating evapotranspiration using TSEB was assessed. Other data, like meteorological, is the same for both simulations. We want to see how the quality of the thermal data, resolution and accuracy, affects the result of TSEB. This study is necessary to determine the minimum requirements of a thermal imagery dataset, suitable for this use-case. The final aim is to improve water productivity and improve yield by early detection of water stress in crops, before it becomes visible.

How to cite: Yadollahi, S. and Tychon, B.: The effect of thermal image quality on the estimation of Crop Evapotranspiration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18886, https://doi.org/10.5194/egusphere-egu26-18886, 2026.

EGU26-19440 | ECS | Orals | GI4.5

TIR Remote Sensing of Volcanic Systems: Recent Advances and Future Perspectives 

Simone Aveni, Gaetana Ganci, and Diego Coppola

Thermal InfraRed (TIR; 10-12 μm) remote sensing provides a robust means to quantify Earth’s emitted radiation, enabling the characterisation of surface thermal state and properties. In volcanic environments, these parameters are directly linked to subsurface processes, energy transfer mechanisms, and eruptive dynamics. However, continuous ground-based monitoring is often impractical, especially in remote or inaccessible regions, due both to logistic constraints and hazardous conditions. As a result, satellite-based thermal observations frequently represent the only viable source of systematic, long-term monitoring.

Volcanic heat flux constitutes a fundamental constraint on volcanic processes and eruption dynamics, yet its estimation from space remains incomplete. Current satellite-based retrievals are largely biased toward Mid-InfraRed (MIR; 3.5-4.5 μm) channels, which are well suited for detecting high-temperature eruptive phenomena. When applied to moderate- and low-temperature volcanic processes, however, MIR-based methods underestimate radiative outputs by up to ~90%, limiting their ability to characterise and quantify hydrothermal activity, unrest, eruptive state transitions, and post-eruptive dynamics.

Recent advances in TIR sensor performance, data availability, and processing capabilities have renewed interest in the TIR domain, demonstrating that TIR observations are not merely complementary to MIR data but essential for capturing a wider spectrum of volcanologically relevant parameters.

Here, we illustrate the advantages of TIR-based approaches for volcano monitoring and present recent methodological advances in TIR data processing, from the use of a dedicated hotspot detection algorithm (TIRVolcH) to retrieve spatially resolved quantitative information, to the application of the recently proposed TIR-based Volcanic Radiative Power (VRPTIR) for quantifying energy release from selected targets and assessing their behaviour. We then show that the synergistic integration of TIR and MIR observations enables discrimination among volcanic features and processes, timely detection of eruptive state transitions, and revision of global volcanic radiative budgets by a factor of 2-20.

How to cite: Aveni, S., Ganci, G., and Coppola, D.: TIR Remote Sensing of Volcanic Systems: Recent Advances and Future Perspectives, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19440, https://doi.org/10.5194/egusphere-egu26-19440, 2026.

EGU26-19538 | ECS | Orals | GI4.5

Extracting Thermal Patterns in Volcanic Areas from Thermal Infrared Satellite Data: A Case Study at the Campi Flegrei Caldera  

Francesco Mercogliano, Andrea Barone, Raffaele Castaldo, Luca D'Auria, Malvina Silvestri, Enrica Marotta, Rosario Peluso, and Pietro Tizzani

In volcanic regions, Thermal InfraRed (TIR) remote sensing is a well-established technique for detecting ground thermal anomalies. The analysis of thermal properties, particularly of Land Surface Temperature (LST) time series, represents a valid tool to achieve a rapid characterization of the shallow thermal field, supporting ground-based surveillance networks in the monitoring of volcanic activity, especially in areas that are inaccessible due to high volcanic hazard.

However, in complex active volcanic and hydrothermal settings, the coexistence of processes of different natures that interact and mutually interfere can significantly affect the distribution of the LST parameter, making it challenging to interpret its spatio-temporal variations. In this context, the extraction of the main thermal patterns of volcanic areas from satellite-derived LST time series represents a further step for a more detailed characterization of the shallow thermal field.

In this study, the extraction of the main thermal patterns from satellite-derived LST time series is addressed through decomposition techniques such as the Independent Component Analysis (ICA) and the Dynamic Mode Decomposition (DMD). ICA is a statistical method aimed at identifying a linear transformation of the data that maximizes the statistical independence between its components, defining the signal’s independent components (ICs). DMD is a data-driven technique aimed at decomposing spatio-temporal data for the extraction of coherent features, defining a set of dominant dynamic modes (DMs). 

The investigated area is the Campi Flegrei caldera (southern Italy), a well-known complex volcanic system. The LST time series is retrieved from cloud-free nighttime TIR images acquired by Landsat-8 and Landsat-9 missions (L8 and L9) during the 2018–2025 time interval. Specifically, the LST parameter is estimated through the Radiative Transfer Equation (RTE) applied to a single thermal band (Band 10 for both L8 and L9) and with known information on the surface emissivity and atmospheric conditions of the investigated area. Subsequently, the application of ICA and DMD methods allowed the identification of the main components, revealing the dominant thermal patterns influencing the LST distribution and providing insights into the endogenous and exogenous processes characterizing the volcanic site.

How to cite: Mercogliano, F., Barone, A., Castaldo, R., D'Auria, L., Silvestri, M., Marotta, E., Peluso, R., and Tizzani, P.: Extracting Thermal Patterns in Volcanic Areas from Thermal Infrared Satellite Data: A Case Study at the Campi Flegrei Caldera , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19538, https://doi.org/10.5194/egusphere-egu26-19538, 2026.

EGU26-19941 | ECS | Orals | GI4.5

Estimating for Subsurface Temperature in the Arctic: Study Case in the Miellajokka Catchment, Northern Sweden 

Romain Carry, Laurent Orgogozo, Yassine ElKhanoussi, Erik Lundin, and Jean-Louis Roujean

Context & Objectives: The northern lands are experiencing a generalised increase in soil temperature, resulting in permafrost thaw and subsequent fast changes on water, heat and matter fluxes in these areas. This triggers many important consequences, including infrastructures destabilisation and release of greenhouse gases. Spaceborne thermal imaging can provide extensive and high-resolution information about the temperature of the arctic continental surfaces. Providing subsurface temperature maps at the scale of a catchment and understanding its interactions with the surface conditions is highly needed for studies of the climate warming induced arctic changes, including permafrost thawing.

Methods: In this study, we used downscaled meteorological data from Nordic Gridded Climate Dataset (NGCD), topographic maps, a land cover map of the region derived from Sentinel-1 and Sentinel-2 data and downscaled Sentinel-3 Land Surface Temperature (LST) images. These surface conditions were combined through a regression model with ten stations of in situ soil-temperature and water content observations positioned along an altitudinal gradient across the Miellajokka watershed, Abisko, Northern Sweden.

Results: We generated soil temperature surface maps for the Abisko region, covering an area of about 52 km² at 300 m spatial resolution. We studied the behaviour of top-layer soil temperature according to climatic conditions, water content, soil properties and surface vegetation.

Conclusion: The developed methodology aims at allowing using satellite images, as thermal observations, for deriving key information about soil thermal regime in the Arctics. By developing this kind of approach, the arctic science community may get tremendous benefit from the future launching of high-resolution TIR observation missions such as TRISHNA and LSTM, for instance for permafrost modelling and climate change impacts assessment.

How to cite: Carry, R., Orgogozo, L., ElKhanoussi, Y., Lundin, E., and Roujean, J.-L.: Estimating for Subsurface Temperature in the Arctic: Study Case in the Miellajokka Catchment, Northern Sweden, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19941, https://doi.org/10.5194/egusphere-egu26-19941, 2026.

EGU26-20029 | Orals | GI4.5

Warming ecosystems in complex terrain – insights from four years of thermal infreared research in the Swiss bio-hydro-cryo spheres  

Kathrin Naegeli, Jennifer Susan Adams, Gabriele Bramati, Alexander Damm, Daniel Odermatt, Abolfazl Irani Rahaghi, Nils Rietze, Gabriela Schaepman-Strub, and Michael Schaepman

Switzerland is among the regions experiencing the strongest warming trends in Europe, with air temperatures increasing well above the global mean. This amplified warming leads to heat stress across terrestrial, aquatic, and cryospheric ecosystems, affecting water availability, ecosystem functioning, and land–atmosphere energy exchange. Capturing these processes requires observations that directly resolve surface temperature dynamics at high spatial and temporal resolution.

Thermal Infrared (TIR) remote sensing has emerged as a key approach to address this need, particularly in light of upcoming satellite missions such as ESA LSTM, CNES/ISRO TRISHNA and NASA SBG-TIR. Over the past four years, different ecosystems in Switzerland have served as testbeds for advancing TIR-based ecosystem research within the ESA PRODEX-funded TRISHNA – Science and Electronics Contribution (T-SEC) project.  

This contribution synthesises scientific insights gained from T-SEC, highlighting recent methodological and instrumental advancements in thermal remote sensing. Key developments include modelling of thermal directionality, advances in calibration and validation strategies, and the use of field campaigns and laboratory measurements to better quantify uncertainties in TIR observations at different spatial, temporal, and spectral scales.  

The presented work spans a range of contrasting ecosystems, including Swiss forests, alpine glaciers and permafrost sites, and perialpine and alpine lakes.  Together, these case studies illustrate the potential and challenges of TIR remote sensing for monitoring ecosystem heat stress, water status, and energy fluxes – always with a particular focus on complex terrain. The results underline the importance of multi-scale, multi-sensor approaches to accurately retrieve surface temperature information. Such information is crucial for understanding ecosystem responses to a rapidly warming climate and for fully exploiting the capabilities of next-generation thermal satellite missions. 

How to cite: Naegeli, K., Adams, J. S., Bramati, G., Damm, A., Odermatt, D., Irani Rahaghi, A., Rietze, N., Schaepman-Strub, G., and Schaepman, M.: Warming ecosystems in complex terrain – insights from four years of thermal infreared research in the Swiss bio-hydro-cryo spheres , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20029, https://doi.org/10.5194/egusphere-egu26-20029, 2026.

Studying the thermal behavior of structures in outdoor conditions, using thermal infrared thermography coupled with local temperature and heat flux probes, is a multidisciplinary field of research and development. It requires to address: system design, informatics, infrared radiometry, signal and image processing, heat transfer and inverse problems domains. In the present study, we present an instrumentation solution system developed in our team to address the remote monitoring of structures in outdoor conditions and its data management. Online infrared measurement corrections, for instance due to variable atmospheric conditions at ground level, are made by using a local weather station equipped with a pyranometer. In case of failure, alternative opportunistic solutions were investigated (Toullier and Dumoulin, 2024), and various strategies of measurements corrections were studied. Comparison of surface temperature measured by infrared thermography and local probes requires to identify the emissivity of materials in the spectral bandwidth used. Such measurements can be made in laboratory but also, when studied surfaces are accessible, by using a portable emissometer. Preliminary results obtained with a 4 spectral band portable emissometer prototype, on a hybrid solar road mock-up deployed in outdoor conditions, will be presented and discussed. To complete, management of acquired data will be presented and discussed in a long term monitoring view. Conclusions on results obtained with a focus on uncooled thermal infrared data will be proposed. Perspectives will address both monitoring system but also recent progress in uncooled infrared sensors (see for instance https://project-brighter.eu/) and temperature emissivity separation algorithms (Toullier et al., 2025) for ground based monitoring systems.

References

  • Toullier, J. Dumoulin, "Bias and bottlenecks study in outdoor long term thermal monitoring by infrared thermography: Leveraging opportunistic data for temperature estimation", Infrared Physics & Technology Journal, Volume 141, August 2024, 105471. https://doi.org/10.1016/j.infrared.2024.105471
  • Toullier, J. Dumoulin, L. Mevel "New joint estimation method for emissivity and temperature distribution based on a Kriged Marginalized Particle Filter: Application to simulated infrared thermal image sequences", Science of Remote Sensing (2025), doi:. https://doi.org/10.1016/j.srs.2025.100209

Acknowledgments

The authors thank ANR (French National Research Agency) for supporting part of this work under Grant agreement ANR-21-CE50-0029-23 and BRIGHTER project. BRIGHTER project has received funding from the Chips Joint Undertaking (Chips JU) under grant agreement N°101096985. The JU receives support from the European Union’s Horizon Europe research and innovation program and France, Belgium, Portugal, Spain, Turkey

How to cite: Dumoulin, J., Toullier, T., and Manceau, J.-L.: Remote monitoring of structures by uncooled thermal infrared thermography coupled with local probes and a data management supervisor, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20500, https://doi.org/10.5194/egusphere-egu26-20500, 2026.

Urban heat islands and extreme heat events are intensifying due to climate change, especially in densely built environments. Remote sensing of land surface temperatures (LST) offers valuable insights for analyzing and mitigating urban heat risks. However, a major limitation of satellite-derived LST data is the trade-off between spatial and temporal resolution. High-resolution products such as those from Landsat provide fine spatial detail but suffer from low temporal coverage, limiting their usefulness for time-critical analyses.

In this study, multiple machine learning approaches are presented to reconstruct high-resolution urban LST data in sub-daily time steps by bridging temporal gaps using observations from the ECOSTRESS sensor on board the ISS. Using Madrid as a case study, random forest, gradient boosting, and artificial neural network models were trained on ECOSTRESS LST data together with a comprehensive set of explanatory variables, including local weather and radiation measurements, ERA5 reanalysis data, and Sentinel-2 surface reflectance indices.

Results show that the different model architectures exhibit varying strengths and weaknesses. The precision of the reconstructions varies with land use; urban areas tend to be reconstructed more accurately than non-built-up, sparsely vegetated areas. Comparing each model’s strengths and weaknesses highlights the potential use of data-driven methods to overcome observational limitations and generate continuous, high-resolution thermal datasets across the diurnal cycle.

By investigating the use of machine learning techniques for the reconstruction of Madrid’s land surface temperature, this work shows a potential pathway to overcome data gaps in high-resolution data on a broader scale. Therefore, it contributes a step toward continuous land surface temperature data, which may help improve the understanding of local heat waves and possible adaptation strategies.

How to cite: Richter, E. and Leuchner, M.:  Reconstructing Urban Surface Temperatures: A Machine Learning Approach to Bridging Temporal Gaps in High-Resolution Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20806, https://doi.org/10.5194/egusphere-egu26-20806, 2026.

EGU26-21199 | Posters on site | GI4.5

Multi-sensor UAS surveys for rapid volume estimation and geomorphological mapping: the July 2024 eruptive crisis at Stromboli volcano 

Nicola Angelo Famiglietti, Maria Marsella, Mauro Coltelli, Enrica Marotta, Antonino Memmolo, Angelo Castagnozzi, Matteo Cagnizi, Peppe J.V. D’aranno, Luigi Lodato, and Annamaria Vicari

The July 4–12, 2024 eruption of Stromboli volcano produced significant effusive activity, pyroclastic density currents and a paroxysmal explosion on July 11, resulting in rapid and substantial morphological changes along the Sciara del Fuoco slope and the summit crater terrace. In this work, we present a quantitative assessment of erupted volumes and associated geomorphological modifications derived from multi-temporal Unmanned Aircraft System (UAS) surveys acquired before, during and after the eruptive sequence.

High-resolution Digital Surface Models (DSMs) and co-registered visible and thermal infrared (TIR) orthomosaics, collected between October 2022 and July 2024, were analysed to reconstruct the evolution of lava flows, erosional features and collapse structures. The integration of TIR data proved essential for identifying active eruptive vents and discriminating cooling lava flows from the complex background of the Sciara del Fuoco. Lava volumes were estimated through a combination of DSM differencing and cross-sectional analyses along the main lava channel, integrating pre-eruptive (May 2024), syn-eruptive (11 July 2024) and post-eruptive (18 July 2024) datasets. TIR surveys provided the thermal constraints necessary to isolate distinct contributions from multiple eruptive vents were quantified, allowing a precise separation of early short-lived lava flows from sustained effusive activity preceding and following the paroxysmal explosion.

Results indicate a total subaerial lava volume of approximately 1.3 × 10⁶ m³ (±20%), with the largest contribution associated with lava emitted from vents located within the central channel. A substantial fraction of this volume formed a lava delta at the coastline, implying the presence of an equivalent or larger submerged deposit. DSM comparisons and thermal anomalies also reveal major erosional processes, including the re-excavation of a pre-existing canyon with an estimated material removal of up to ~5 × 10⁶ m³, and a summit area collapse producing a depression of 70–90 m and a missing volume of ~1.9 × 10⁶ m³.

These results highlight the effectiveness of rapid multi-sensor UAS-based surveying for near-real-time volume estimation and morphodynamic analysis during volcanic crises. This approach provides key constraints for mass balance assessments, hazard evaluation and coastal instability monitoring at active volcanoes such as Stromboli.

How to cite: Famiglietti, N. A., Marsella, M., Coltelli, M., Marotta, E., Memmolo, A., Castagnozzi, A., Cagnizi, M., D’aranno, P. J. V., Lodato, L., and Vicari, A.: Multi-sensor UAS surveys for rapid volume estimation and geomorphological mapping: the July 2024 eruptive crisis at Stromboli volcano, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21199, https://doi.org/10.5194/egusphere-egu26-21199, 2026.

EGU26-21467 | Posters on site | GI4.5

Enabling Rapid Thermal Infrared (TIR) Monitoring in Restricted Airspaces: U-space Integration for and Environmental Assessment 

Gala Avvisati, Enrica Marotta, Orazio Colucci, Simone Menicucci, and Andrea Barone

High-frequency Thermal Infrared (TIR) observations are essential for characterizing surface temperature anomalies in areas exposed to natural and anthropogenic hazards. However, in densely urbanized regions like Southern Italy, airspace restrictions often delay UAS deployments, hindering real-time data collection during evolving crises. This study explores the integration of UAS within the U-space ecosystem—including network identification and geo-awareness—as a transformative enabler for advanced thermal remote sensing.

We present multidisciplinary case studies in the Campania Region where TIR payloads on UAS platforms were successfully employed for: 1) identifying thermal anomalies in the Campi Flegrei caldera; 2) detecting persistent soil moisture and flood causes in agricultural areas; and 3) assessing fire ignition risks in illegal waste disposal sites; 4) definition of susceptibility maps for the triggering of anthropogenic sinkholes. By overcoming "no-fly zone" limitations through Unmanned Traffic Management (UTM) experiments, we demonstrate how rapid TIR data acquisition provides crucial decision-making tools for risk management.

To bridge the gap between research, monitoring, and operational continuity, we will launch, in agreement with ENAC, an initial U-Space test on the island of Ischia (characterized by volcanic and hydrogeological multi-hazards) since it currently has fewer airspace restrictions.

How to cite: Avvisati, G., Marotta, E., Colucci, O., Menicucci, S., and Barone, A.: Enabling Rapid Thermal Infrared (TIR) Monitoring in Restricted Airspaces: U-space Integration for and Environmental Assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21467, https://doi.org/10.5194/egusphere-egu26-21467, 2026.

EGU26-22290 | Posters on site | GI4.5

Hydrogeological insights from UAS thermal remote sensing. Case study at Sant'Angelo (Ischia, Italy) 

Silvia Fabbrocino, Enrica Marotta, Gala Avvisati, Pasquale Belviso, Rosario Avino, Eliana Bellucci Sessa, Antonio Carandente, Eugenio Di Meglio, and Rosario Peluso

Thermal Infrared (TIR) remote sensing from Unmanned Aerial Systems (UAS) has revolutionized the monitoring of volcanic and hydrothermal environments, providing a critical link between ground-based observations and satellite data. In coastal volcanic settings, the identification of hydrothermal discharge points—such as hot springs and fumaroles—is often challenged by their intermittent nature and the dynamic interface between the terrestrial and marine domains.

This study presents a high-resolution thermal mapping survey conducted along the Sant'Angelo beach on the island of Ischia (Gulf of Naples, Italy). By leveraging the flexibility and high spatial resolution of UAS-mounted TIR sensors, we successfully identified and characterized localized thermal anomalies that are otherwise undetectable through conventional field surveys or lower-resolution satellite imagery. A key finding of this work is the detection of a distinctive submarine-to-intertidal fumarolic vent that emerges on the shoreline exclusively during low-tide conditions.

From a hydrogeological perspective, the ability to precisely map these "transient" thermal signatures provides crucial insights into the structural control of fluid migration and the spatial distribution of the hydrothermal system’s discharge zones. These thermal features act as preferential pathways for pressurized fluids, and their characterization is fundamental for refining the hydrogeological conceptual model of the Ischia volcanic system. Our research indicates that UAS-TIR mapping has the potential to enhance coastal hydrogeology in volcanic regions by detecting ephemeral thermal targets and enhancing the assessment of geothermal potential and volcanic unrest indicators. This approach offers a cost-effective and non-invasive methodology for monitoring hydrothermal activity at the land-sea interface, with significant implications for both environmental management and geohazard mitigation.

How to cite: Fabbrocino, S., Marotta, E., Avvisati, G., Belviso, P., Avino, R., Bellucci Sessa, E., Carandente, A., Di Meglio, E., and Peluso, R.: Hydrogeological insights from UAS thermal remote sensing. Case study at Sant'Angelo (Ischia, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22290, https://doi.org/10.5194/egusphere-egu26-22290, 2026.

EGU26-22977 | Orals | GI4.5

PROMETHEUS: City-scale material mapping with large vision models for emissivity-based airborne thermography 

Dirk Tiede, Martin Sudmanns, Max Aragon, Jose Gomez, Carla Arellano, Daniel Rüdisser, Sophia Klaußner, and Günter Koren

Deriving land surface temperatures (LST) from aerial thermography requires surface emissivity information, which is typically assumed uniform despite considerable variation across urban materials. We present PROMETHEUS, a workflow that uses a fine-tuned Large Vision Model (LVM) to produce city-scale material classification at airborne resolution. This classification enables emissivity-based LST estimation following the GRAZ method, which uses three-dimensional Monte Carlo sampling to determine view factors for reflected thermal radiation and models elevation-dependent atmospheric transmittance, upwelling and downwelling radiation. We applied this workflow to a 100×100 km area centred on Klagenfurt, Austria, where thermal infrared imagery at 1 m resolution was acquired on August 10-11, 2024 during a summer heat period, with daytime and nighttime flights at 1600 m altitude. A team of 12 surveyors collected concurrent in-situ land and water surface temperatures across 13 stations throughout the city. Using existing 5 cm RGB and near-infrared orthoimagery combined with photogrammetric building segmentation, expert annotators labelled rooftop materials across 30 classes via a collaborative platform with a standardized material guide. These labels were used to fine-tune an LVM that then classified materials across the full study area. The output was merged with municipal land cover data and converted to emissivity values using a look-up table derived from spectral libraries. Atmospheric parameters were obtained from ECMWF profiles. Comparison with in-situ measurements shows improved LST retrieval relative to uniform emissivity assumptions, particularly for low-emissivity surfaces such as metal roofing. This workflow demonstrates a practical approach for scaling limited expert annotations to city-wide material mapping.

How to cite: Tiede, D., Sudmanns, M., Aragon, M., Gomez, J., Arellano, C., Rüdisser, D., Klaußner, S., and Koren, G.: PROMETHEUS: City-scale material mapping with large vision models for emissivity-based airborne thermography, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22977, https://doi.org/10.5194/egusphere-egu26-22977, 2026.

EGU26-631 | ECS | Posters on site | G3.1

Length of Day Variability and Climate Indicators: Insights from ENSO Events  

Dominika Staniszewska and Małgorzta Wińska

The interplay between the length of day (LOD) and the El Niño–Southern Oscillation (ENSO) has been investigated in geophysical research since the 1980s. LOD, defined as the negative time derivative of UT1-UTC, is intrinsically linked to the Earth Rotation Angle (ERA), a fundamental Earth Orientation Parameter (EOP).

ENSO, a dominant climate mode in the tropical eastern Pacific, substantially influences tropical and subtropical regions. Extreme ENSO episodes are associated with significant hydroclimatic anomalies across multiple regions, including severe droughts and floods. These events evolve over extended incubation periods, during which interannual fluctuations in LOD and the angular momentum of the atmosphere (AAM), ocean (OAM), and lithosphere/hydrogeosphere (HAM) are modulated by complex ocean–atmosphere interactions.

Key manifestations of ongoing climate change, such as rising global temperatures and sea levels, are strongly modulated by ENSO. Interannual variability in global mean sea surface temperature (GMST) and global mean sea level (GMSL) further reflects Earth's rotational dynamics changes.

This study aims to elucidate the interannual (2–8 years) couplings between LOD, AAM, OAM, HAM, and selected climate indices, including the Southern Oscillation Index (SOI), Oceanic Niño Index (ONI), GMST, and GMSL. The influence of these climate signals on LOD from 1976 to 2024 will be assessed using advanced semblance analysis, exploring multiple methodological variants based on the continuous wavelet transform to capture correlations across both temporal and spectral domains.

A detailed understanding of these interactions enhances our knowledge of Earth’s dynamic system, informs geophysical modeling efforts, and improves the precision of applications that rely on accurate timekeeping and measurements of Earth’s rotational behaviour. 

How to cite: Staniszewska, D. and Wińska, M.: Length of Day Variability and Climate Indicators: Insights from ENSO Events , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-631, https://doi.org/10.5194/egusphere-egu26-631, 2026.

EGU26-4049 | Posters on site | G3.1

Estimation of surface hydrological diffusivity and atmospheric flux bias using GRACE satellite data 

Guillaume Ramillien, José Darrozes, and Lucia Seoane

Variations in terrestrial water storage (TWS), as observed by the GRACE/GRACE-FO  missions, provide unique insights into large-scale hydrological processes. However, translating these satellite observations into transport parameters such as surface diffusivity, lateral water fluxes, and groundwater recharge remains challenging. In this study, we propose using a surface diffusion-advection model coupled with a WGHM data assimilation framework of gridded GRACE solutions to estimate subsurface diffusivity and systematic precipitation–evapotranspiration biases simultaneously. The global kinematic hydrology model represents the lateral and vertical transport of water by diffusion, while GRACE observations represent the total water storage. In the steepest descent 4D Var-like procedure, the parameter gradients of the objective function are computed using the hydrological model's adjoint. Errors on derived diffusivities are also computed. The optimised parameters enable us to diagnose effective surface diffusivity and lateral water fluxes, as well as net groundwater recharge. This framework provides a physically consistent interpretation of GRACE-observed mass redistribution and offers new perspectives on large-scale hydrological transferts.

How to cite: Ramillien, G., Darrozes, J., and Seoane, L.: Estimation of surface hydrological diffusivity and atmospheric flux bias using GRACE satellite data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4049, https://doi.org/10.5194/egusphere-egu26-4049, 2026.

More than 90% of the excess energy entering the Earth system due to increased greenhouse gas concentrations is stored in the ocean within just a few years. This ocean heat storage has helped limit surface warming and modulate Earth’s radiative response, thereby influencing the global energy budget. Understanding Ocean Heat Content (OHC), including its temporal and spatial variations, is crucial for grasping global energy dynamics and constraining climate change projections.

Geodetic observations from satellite gravimetry (GRACE and GRACE-FO) and satellite altimetry enable to estimate OHC through thermal expansion, derived from sea level rise corrected for changes in ocean mass. This geodetic approach provides broad coverage and high resolution but faces challenges in resolving interannual variability. In particular, it cannot determine the depth at which heat is stored, introducing ambiguity when converting thermal expansion into OHC anomalies.

This work introduces a new OHC product that, for the first time, combines in-situ, altimetric, and gravimetric data using an inverse method. The inclusion of in-situ ARGO data helps constrain the vertical distribution of heat down to 2000 m, addressing ambiguities in the geodetic approach. By optimizing the residuals between in-situ and geodetic OHC and applying objective mapping techniques, the method produces consistent OHC fields along with associated uncertainty estimates.

The new product is validated against existing in-situ datasets. Its derivative—Ocean Heat Uptake (OHU)—is compared with CERES radiation budget data to assess the closure of the Earth’s energy balance over the ocean. The comparison shows that the ocean energy budget is closed from the top of the atmosphere (TOA) to 2000 m depth on an annual basis, with a residual of approximately 0.3 W/m² (1σ). This implies that energy anomalies greater than 0.3 W/m² can be tracked within the ocean system between TOA and 2000 m depth thanks to their signature on the Earth deformation.

How to cite: Blazquez, A., Meyssagnac, B., Fourest, S., and Duvignac, T.: Satellite gravimetry and altimetry combined with in-situ ocean temperature profiles enable to close the Earth energy budget and track yearly global energy anomalies from top of the atmosphere to the ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6539, https://doi.org/10.5194/egusphere-egu26-6539, 2026.

Coastal zones face increased risks from the combined effects of climate-driven sea-level rise and vertical land motion (VLM), which together determine rates of relative sea-level (RSL) change. While oceanic contributions to RSL are increasingly well monitored and projected, land subsidence (i.e., negative VLM) remains one of the least systematically observed and most spatially heterogeneous components of RSL, despite its potential to locally exceed climate-driven ocean rise by an order of magnitude. This observational gap is especially pronounced in rapidly urbanizing and data-limited regions, where sparse tide-gauge and GNSS networks hinder the identification of subsidence hotspots and their evolving impacts on coastal risks.

In this talk, I present a framework that leverages satellite geodesy as a climate observing system to resolve the spatiotemporal dynamics of land subsidence and quantify its contribution to present and future relative sea-level change, using Java Island, Indonesia, as a regional-scale case study. We generated high-spatial resolution (75 m) contemporary VLM fields from using multi-geometry Sentinel-1 interferometric synthetic aperture radar (InSAR), revealing widespread and temporally evolving subsidence patterns with rates exceeding 1 cm per year across multiple coastal and inland urban centers. While Jakarta has dominated the subsidence narrative in Indonesia, we find that several other coastal cities, including Cirebon, Pekalongan, Tegal, and Semarang, are sinking two to three times faster, with localized rates approaching 10 cm per year.

To disentangle the dominant drivers of deformation, we applied unsupervised machine-learning spatiotemporal clustering to InSAR time series, guided by geological and land-use information. This analysis reveals nonlinear and spatially heterogeneous subsidence behaviors primarily associated with groundwater extraction in urban, industrial, and agricultural regions, alongside localized deformation linked to natural processes such as volcanism. Finally, we constructed synthetic tide-gauge records at 5-km spacing along the 1,500 km northern coastline by integrating InSAR-derived VLM with satellite altimetry and probabilistic sea-level projections. These virtual gauges show that neglecting land subsidence leads to systematic underestimation of RSL change by more than 90% in some locations and that subsidence will remain the dominant contributor to RSL rise across much of the coastline through 2050.

This work illustrates how geodetic observing systems can fill critical observational gaps in coastal climate research, enabling spatially explicit, process-informed RSL estimates and providing a transferable framework for improving sea-level risk assessments in vulnerable, data-sparse regions worldwide.

How to cite: Ohenhen, L.: Resolving land subsidence contribution to present and future relative sea level change using satellite geodesy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8826, https://doi.org/10.5194/egusphere-egu26-8826, 2026.

EGU26-9263 | ECS | Orals | G3.1

Scientific Scenarios of Climate Change for Decadal Forecasts of Earth’s Surface Movements in Germany  

Nhung Le, Anna Klos Kłos, T.T.Thuy Pham, T.Thach Luong, Chinh Nguyen, and Maik Thomas

Abstract:

Climate change has been proven to exacerbate the ongoing deformations of the Earth's surface in Germany. Also, human activities such as mining, fluid extraction, and reservoir-induced seismicity cause local surface deformations. Therefore, long-term forecasts of Earth's surface movements are needed for infrastructure planning, hazard mitigation, and the sustainable management of natural resources in Germany. By applying Machine Learning (ML) and statistical analyses, we develop scientific scenarios of climate change to forecast surface movements in Germany over the next two decades. Together with Global Navigation Satellite Systems (GNSS), data from five interdisciplinary fields, including the Sun and Moon ephemerides, polar motions, surface loadings, gravity variations, and meteorology, are utilized as features for training ML-based forecast models. Our results indicate that the accuracy of regression ML models reaches millimeter levels, and the decadal forecast models produce fewer than 2% extreme values in the total predictions per year. Based on climate change scenarios, the findings reveal that the average intra-plate motions in Germany will accelerate from ~1.2 mm/yr to ~1.5mm/yr over the next two decades. The annual variations across the 346 GNSS monitoring stations are predicted to increase from 4.7mm to 5.1mm. Surface deformations will be more severe in the southeastern regions and river basins such as the Elbe, Weser, Ems, and Rhine. Significant extensions are expected in the Eifel volcanic region, while notable compressions may occur along the Upper Rhine Graben and the Saxony region in the next twenty years. Additionally, experimental functions showing the statistical distribution of Earth's surface deformation trends in Germany over the next two decades have been proposed. Potentially, the methodology in this study can also be adapted to forecast surface movements related to climate change in polar regions.

Keywords:

Climate change, Surface deformation, Movement forecast, Machine learning, GNSS

How to cite: Le, N., Kłos, A. K., Pham, T. T. T., Luong, T. T., Nguyen, C., and Thomas, M.: Scientific Scenarios of Climate Change for Decadal Forecasts of Earth’s Surface Movements in Germany , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9263, https://doi.org/10.5194/egusphere-egu26-9263, 2026.

EGU26-9761 | ECS | Posters on site | G3.1

A study of the potential for using trends of GPS displacements to determine TWS trends in Poland 

Kinga Kłos, Anna Klos, and Artur Lenczuk

Permanent stations of the Global Positioning System (GPS) enable the registration of elastic deformations of the Earth’s surface that occur in response to variations in hydrological mass loads over continental areas. Analysis of long-term changes in displacements observed by a set of GPS permanent stations allows for the identification of deformations induced by long-term changes of the Terrestrial Water Storage (TWS). Densely distributed GPS stations provide adequate spatial coverage for regional scale analysis and their exact spatio-temporal analysis. We use a set of vertical displacements for the period 2010-2020 observed by 493 GPS permanent stations situated in Poland and neighboring regions, whose observations were processed by the Nevada Geodetic Laboratory (NGL). 213 of these stations exhibit more than 80% of temporal coverage with Gravity Recovery and Climate Experiment (GRACE) and GRACE Follow-On satellite missions. We use these vertical displacements and invert them using elastic Earth theory and load Love numbers to infer trends of TWS in Poland. The obtained results were compared with independent estimates of TWS trends derived from the GRACE and GRACE Follow-On missions, and other external datasets. The analysis demonstrates that GPS-observed vertical displacements provide a reliable source of information for the assessment of TWS trends in Poland.

How to cite: Kłos, K., Klos, A., and Lenczuk, A.: A study of the potential for using trends of GPS displacements to determine TWS trends in Poland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9761, https://doi.org/10.5194/egusphere-egu26-9761, 2026.

EGU26-10722 | ECS | Orals | G3.1

Benefits of future satellite gravimetry missions for characterizing extreme wet events in terrestrial water storage 

Klara Middendorf, Laura Jensen, Marius Schlaak, Julian Haas, Henryk Dobslaw, Roland Pail, Andreas Güntner, and Annette Eicker

Under the assumption that a warming climate leads to an intensification of the global water cycle, it is hypothesized that also the occurrence frequency and severity of extreme events such as droughts and floods will increase in the upcoming decades. GRACE/-FO observations of terrestrial water storage (TWS) have been used in the past to identify and analyse extreme events both on a global and regional scale. However, these analyses are restricted by the limited spatial and temporal resolution of current satellite gravimetry observations. Especially, flooding events tend to occur very locally and with short temporal (sub-monthly) extent, thus capturing them is challenging. Future satellite gravimetry missions, particularly the double-pair constellation MAGIC, are expected to significantly enhance the spatial and temporal resolution. In this study, we globally investigate the benefit MAGIC can achieve to detect wet extreme events using long-term (50 years) end-to-end simulations of GRACE-C and MAGIC.

The simulation environment is based on the acceleration approach and considers tidal and non-tidal background model errors as well as instrument noise of the acceleration and ranging instruments following the current MAGIC mission design studies. As input and reference, we use the daily output of a climate model (GFDL-CM4) from the CMIP6 archive that has been identified as a realistic representation of water storage evolution in previous studies. To explore the improved temporal and spatial resolution expected from the MAGIC constellation, we (i) compare extreme values derived from 5-daily gravity field simulations to those from monthly fields, and (ii) show how the weaker spatial filtering required for MAGIC has a positive influence on the detectability of extremes.

For the analysis two different approaches are exploited: One method focuses solely on the stochastic characteristics of the time series in terms of extreme value theory, evaluating the magnitude-frequency relationship of large TWS values by calculating expected return levels of wet extremes. The other approach builds on the fact that a 50-years simulation time series allows to derive statistically meaningful conclusions from directly comparing reference and simulation output on a time series level. We evaluate the time of occurrence of wet extremes on the basis of classification scores assessing correctly and incorrectly identified extreme events.

How to cite: Middendorf, K., Jensen, L., Schlaak, M., Haas, J., Dobslaw, H., Pail, R., Güntner, A., and Eicker, A.: Benefits of future satellite gravimetry missions for characterizing extreme wet events in terrestrial water storage, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10722, https://doi.org/10.5194/egusphere-egu26-10722, 2026.

EGU26-10826 | ECS | Orals | G3.1

A global inversion for sea-level contributions from satellite data: towards improving Antarctica's representation 

Matthias O. Willen, Bernd Uebbing, Martin Horwath, and Jürgen Kusche

Variations in sea level are a globally comprehensively measurable indicator of the effect of climate change on the Earth system. Satellite geodesy provides data with global coverage to analyze sea level changes in space and time, but also to investigate the individual contributions to sea level from the subsystems oceans, continental hydrology, glaciers, ice sheets, and the solid Earth. Particularly valuable for this purpose are time-variable satellite gravity, realized by the GRACE and GRACE-FO missions, and satellite altimetry over the oceans, realized, e.g., by the Jason-1/-2/-3 and Sentinel-6 reference missions. However, previous studies show that the uncertainty of the estimated Antarctic Ice Sheet’s contribution to sea level remains large, primarily due to errors in the glacial isostatic adjustment (GIA) correction. We use a global fingerprint inversion method that evaluates GRACE and ocean altimetry data in a globally consistent framework and enables the quantification of individual contributions to sea level on a monthly basis on global grids. The inversion is additionally supplemented by observations from Argo floats. The parametrization of the contributions from steric effects, ice sheets, glaciers, hydrology, and GIA are realized by time-invariant sea-level fingerprints obtained from a priori information. This includes, e.g., the locations of mass changes or statistically obtained information from geophysical model simulations. In a methodological advancement of the inversion method, we have implemented a new parametrization of the ice mass changes (IMC) of the Antarctic ice sheet. Previously, IMC and corresponding sea level change has been estimated only on basin level for 27 large ice catchment areas, so-called drainage basins. However, this coarse parametrization of IMC prevents the inversion method from better resolving errors in the GIA correction in upcoming inversion implementations. We have therefore introduced a high-resolution parametrization based on individual grid points with a resolution of up to 50 km, resulting in up to 4755 Antarctic mass balance parameters to be estimated in a globally consistent way. In order to solve this inverse problem, we introduced altimetry over ice sheets as an additional observation at a 10 km spatial and a monthly temporal resolution. We present and discuss results from different variants of parametrization of IMC and different variants of implementation of ice altimetry observations. This methodological advancement presented here is a necessary step towards minimizing GIA-related errors when determining the sea level budget utilizing this global framework in the future.

How to cite: Willen, M. O., Uebbing, B., Horwath, M., and Kusche, J.: A global inversion for sea-level contributions from satellite data: towards improving Antarctica's representation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10826, https://doi.org/10.5194/egusphere-egu26-10826, 2026.

EGU26-10838 | ECS | Posters on site | G3.1

Impact of non-tidal loading corrections and processing strategy on Antarctic GNSS vertical time series 

Aino Schulz, Yohannes Getachew Ejigu, Jyri Näränen, and Maaria Nordman

Accurate estimation of vertical land motion in Antarctica is crucial for understanding glacial isostatic adjustment (GIA), ice mass change, and sea-level rise. However, Global Navigation Satellite System (GNSS) position time series are affected by non-tidal loading (NTL), which can obscure geophysical signals and bias trend estimates. In this study, we evaluate the performance of 11 NTL model combinations from EOST (École & Observatoire des Sciences de la Terre, Strasbourg) and ESMGFZ (Earth System Modelling Group, GFZ Potsdam) in correcting vertical GNSS time series at three East Antarctic stations in Dronning Maud Land. We analyse five GNSS solutions processed with different strategies, including precise point positioning (PPP), double-difference (DD) network solutions, and a combined product.

Our results show that NTL corrections improve time series quality in PPP-based solutions, reducing root mean square (RMS), coloured noise, and seasonal amplitudes by more than 20 % at some sites. In contrast, network-based and combined solutions exhibit limited improvements, and in some cases, corrections introduced additional variability. Among loading components, non-tidal atmospheric loading (NTAL) consistently produces the largest reductions, while additional non-tidal oceanic (NTOL) and hydrological loading (HYDL) contributions are beneficial mainly in specific GFZ model combinations applied to PPP datasets.

Our findings demonstrate that both GNSS processing strategy and NTL model choice can affect inferred vertical trends, and in some cases even change their sign. Our evaluation provides a regional assessment of widely used NTL products under Antarctic conditions, with direct implications for GIA modelling and reference frame realisation, and supports the development of more robust correction strategies for future Antarctic GNSS studies.

How to cite: Schulz, A., Ejigu, Y. G., Näränen, J., and Nordman, M.: Impact of non-tidal loading corrections and processing strategy on Antarctic GNSS vertical time series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10838, https://doi.org/10.5194/egusphere-egu26-10838, 2026.

EGU26-10903 | Posters on site | G3.1

Multi-year regional water mass solutions by inversion of hydrology-related GRACE(-FO) KBRR residuals 

Lucia Seoane, Guillaume Ramillien, and José Darrozes

Our analysis presents 10-day water mass solutions estimated from both GRACE and GRACE-FO KBR Range (KBRR) residuals for continental hydrology using GINS software developed by the CNES/GRGS group.  The inter-satellite velocity residuals have been converted into along-track differences of gravity potential using the energy balance approach. Maps of Equivalent Water Height (EWH) are obtained by inversion of these potential differences onto juxtaposed surface elements over the region of interest or time coefficients of designed orthogonal Slepian functions. This latter band-limited representation offers the advantage of reducing  drastically the number of parameters to be fitted and the computation time. We also used another type of orthogonal basis functions, as well as decomposition using anisotropic wavelets. These functions require larger computing resources but have the advantage of being adapted to the shape of the studied watersheds for improving hydrology variation survey locally. All of these regional solutions are compared to spherical harmonics and mascons series of existing Level-2 solutions for validation. The patterns shown in the proposed regional solutions reveal dominant seasonal cycles of water mass in the large tropical basins (e.g. Amazon,  Nil and Congo), as well as extreme events such as floods and droughts.

How to cite: Seoane, L., Ramillien, G., and Darrozes, J.: Multi-year regional water mass solutions by inversion of hydrology-related GRACE(-FO) KBRR residuals, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10903, https://doi.org/10.5194/egusphere-egu26-10903, 2026.

EGU26-11806 | ECS | Orals | G3.1

TUD-L2B-EWH_UNC: A Monthly Global Level-2B GRACE(-FO) EWH Uncertainty Product 

Michal Cuadrat-Grzybowski and Joao G. de Teixeira da Encarnacao

The Gravity Recovery and Climate Experiment (GRACE) and its successor GRACE-FO provide unique observations of Earth’s time-variable gravity field, enabling direct monitoring of mass redistribution expressed as equivalent water height (EWH). While gridded Level-2B products are widely used across hydrology, glaciology, and solid-Earth studies, uncertainty information remains fragmented or inaccessible to end users. In practice, this has led to the widespread use of empirical or ad hoc uncertainty estimates, limiting data assimilation and other geophysical applications that require spatially and temporally resolved observational error information.

We present TUD-L2B-EWH_UNC-GRACE, a globally gridded Level-2B GRACE(-FO) EWH data product that provides a comprehensive and transparent characterisation of uncertainty alongside the mass anomaly fields. Unlike conventional approaches that rely on propagation of full normal matrices or impose assumptions on error correlations, TUD-L2B-EWH_UNC combines ensemble statistics from multiple independently processed Level-2 solutions to quantify pre-processing uncertainties. These include contributions from ocean tide model differences, parametrisation strategies, and uncertainty in the Atmosphere and Ocean De-aliasing (AOD1B) background model.

Post-processing uncertainties associated with filtering, leakage, and Glacial Isostatic Adjustment (GIA) are quantified separately. Filtering-related uncertainty is evaluated using a known-pair approach, while GIA uncertainty is assessed using an ensemble of 56 published GIA models. Error fields are provided for a suite of anisotropic filtering strategies (DDK(2–7)), enabling systematic assessment of filtering choices, leakage effects, and model dependence on the total uncertainty budget.

TUD-L2B-EWH_UNC is the first Level-2B EWH dataset to deliver end-to-end, spatially and temporally resolved uncertainty fields in a user-ready gridded format. This design supports consistent uncertainty handling across hydrological, glaciological, and solid-Earth applications. Ancillary tidal corrections and climatological fits of signal and leakage-related errors are distributed separately through the companion products TUD-L2B-EWH_CLIM-GRACE and TUD-L2B-EWH_CLIM_LEAKAGE-GRACE. All datasets are publicly available (DOI: doi.org/10.4121/4fc748e8-01c7-4f06-87da-653937b078f7) via the TU Delft GRACE Portal (https://grace-cube.lr.tudelft.nl/).

How to cite: Cuadrat-Grzybowski, M. and de Teixeira da Encarnacao, J. G.: TUD-L2B-EWH_UNC: A Monthly Global Level-2B GRACE(-FO) EWH Uncertainty Product, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11806, https://doi.org/10.5194/egusphere-egu26-11806, 2026.

EGU26-12466 | ECS | Posters on site | G3.1

Improving the representation of water, energy and carbon cycles in land surface modelling: Assimilation of MAGIC TWSA data 

Annika Nitschke, Jürgen Kusche, and Harrie-Jan Hendricks Franssen

The upcoming MAGIC (Mass Change and Geoscience International Constellation) mission aims to extend the current record of mass change observations with higher spatiotemporal resolution data. This study evaluates the potential of terrestrial water storage (TWS) observations from MAGIC in improving our understanding of the coupled water, energy, and carbon cycles.   

Using a synthetic data assimilation experiment, we integrate simulated MAGIC TWS data into a high-resolution (3 km) land surface model over two European study areas. These regions are selected for their strong land-atmosphere coupling, providing suitable test cases for investigating whether and how improvements in soil moisture profiles and snow cover from TWS assimilation translate to improved estimates in energy and carbon cycle variables. Our research addresses two primary objectives: (i) quantifying the added benefit of assimilating TWS changes in constraining model states, such as land surface temperature and vegetation growth, relative to a known reference, and (ii) investigating how the increased resolution of MAGIC supports an improved representation of land-atmosphere coupling, particularly during extreme drought events, using ecosystem-scale water use efficiency (the ratio of gross primary productivity to evapotranspiration) as a diagnostic of vegetation response. 

How to cite: Nitschke, A., Kusche, J., and Hendricks Franssen, H.-J.: Improving the representation of water, energy and carbon cycles in land surface modelling: Assimilation of MAGIC TWSA data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12466, https://doi.org/10.5194/egusphere-egu26-12466, 2026.

EGU26-12707 | ECS | Posters on site | G3.1

Study of changes induced by global warming in Svalbard based on spatial geodetic data and in situ geophysical measurements 

Alicia Tafflet, Joëlle Nicolas, Agnès Baltzer, Jérome Verdun, Florian Tolle, Eric Bernard, and Jean-Michel Friedt

The Svalbard Archipelago, located in the Arctic region of Norway, is extremely vulnerable to the climate change. With a current increase of 3 at 5°C in average air temperature and a change in precipitation with an increasing proportion of rain, certain negative consequences for the environment and ecosystem are inevitable. One of the most obvious signs of climate change in this region is the melting of ice, which is causing the Earth’s crust to deform. But there are other consequences, such as the loss of sea ice cover, changes in how sediment is transported and also changes in biodiversity.

These phenomena are widely studied in this region. For example, deformation of the Earth’s crust is determined using 3D positioning data acquired by GNSS across Svalbard, particularly  in Ny-Alesund. Since 2000, daily positioning time series show a strong upward component, with an average vertical velocity of between 8 to 13 mm/yr. This velocity is the Earth’s response  to various episodes of glaciation and deglaciation in the past like the last glacial maximum or the Little Ice Age, and to the current melting of ice. This current melting has also been  studied a lot at Ny-Alesund station, where glaciers are monitored to measure changes in ice height from one year to the next and calculate the glacier’s surface mass balance. This is the case for the Austre Lovenbreen, for which data has been available since 2007, showing record melting over the last ten years. The same is true for the study of the prodeltas evolution since 2009, which shows a stabilisation of almost all prodeltas since 2016.

All these phenomena are largely studied separately, but our analysis consists of interpreting all this data in order to study the possible correlation between these observations which share the same cause: climate change. In our study, we ask how we can link measurements taken at the glacier or in the underwater sediment, along with space geodesy data, to better understand the ongoing geophysical processes that mark the transition between a glacial environment and paraglacial environment.

How to cite: Tafflet, A., Nicolas, J., Baltzer, A., Verdun, J., Tolle, F., Bernard, E., and Friedt, J.-M.: Study of changes induced by global warming in Svalbard based on spatial geodetic data and in situ geophysical measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12707, https://doi.org/10.5194/egusphere-egu26-12707, 2026.

EGU26-12852 | ECS | Posters on site | G3.1

Quantifying mass signatures of drought and flood events using water fluxes and terrestrial water storage anomalies 

Sedigheh Karimi, Roelof Rietbroek, Marloes Penning de Vries, and Christiaan van der Tol

The Gravity Recovery and Climate Experiment (GRACE) and its follow-on mission (GRACE-FO) have been providing spaceborne observations of terrestrial water storage (TWS) changes since 2002. These observations help to understand how water fluxes change in an intensifying water cycle at watershed scales. However, the accuracy of the derived TWS anomalies depends on the choice of spatial and spectral filtering methods, which can attenuate their amplitude.

In this poster, we present our filter-free inversion scheme that estimates TWS anomalies at watershed scales from Level-2 Stokes coefficients together with their associated full error covariance matrices. We apply the scheme to the watersheds in the Greater Horn of Africa and compare the obtained TWS anomalies with the accumulated watershed-wide precipitation and evapotranspiration fluxes from the ERA5 atmospheric reanalysis, and the accumulated river discharge from GLOFAS and GEOGLOWS products. We further assess the consistency between the temporal derivatives of TWS anomalies and the corresponding water fluxes. Additionally, we quantify mass deficits and surpluses in TWS anomalies and investigate the relative contributions of atmospheric net flux (i.e., precipitation minus evapotranspiration) and river discharge to the magnitude of TWS anomalies during drought and flood events.

How to cite: Karimi, S., Rietbroek, R., Penning de Vries, M., and van der Tol, C.: Quantifying mass signatures of drought and flood events using water fluxes and terrestrial water storage anomalies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12852, https://doi.org/10.5194/egusphere-egu26-12852, 2026.

EGU26-15089 | ECS | Posters on site | G3.1

Snow Accumulation Monitoring using GNSS-Interferometric Reflectometry for Antarctica 

Laura Crocetti, Christopher Watson, Matthias Schartner, and Matt King

Antarctica plays a central role in Earth's global climate system and stores most of the planet's freshwater. However, due to the continent's remoteness and extreme conditions, reliable in situ observations of snow accumulation remain rare. This gap in measurements makes it difficult to constrain ice sheet models and accurately project Antarctica's contribution to global sea level rise. In particular, regions such as the Totten Glacier in East Antarctica are of interest due to the significant mass loss since the 1990s, dominated by changes in coastal ice dynamics. In the context of Antarctica, GNSS Interferometric Reflectometry (GNSS-IR) presents an efficient and sustainable approach to monitor changes in snow accumulation with the potential to offer insights into regional surface mass balance models.

This contribution investigates a unique in situ dataset of six GNSS stations deployed on the Totten Glacier, operated seasonally between November 2016 and January 2019. These stations were originally designed to track ice motion, but they also capture reflections from the snow surface. By applying GNSS-IR, time series of snow accumulation are generated – once with the traditional retrieval approach using the gnssrefl software, and once by testing a novel machine learning-based retrieval framework. The derived snow accumulation time series are cross-referenced with outputs from regional surface mass balance models. The results provide insights into the spatio-temporal patterns of snow accumulation over the Totten Glacier and showcase the potential of GNSS-IR for environmental sensing.

How to cite: Crocetti, L., Watson, C., Schartner, M., and King, M.: Snow Accumulation Monitoring using GNSS-Interferometric Reflectometry for Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15089, https://doi.org/10.5194/egusphere-egu26-15089, 2026.

EGU26-16019 | ECS | Posters on site | G3.1

Spatially refined global terrestrial water storage trends and annual cycles from GRACE and GRACE-FO 

Mary Michael O'Neill, Matt Rodell, and Bryant Loomis

Satellite gravimetry has revolutionized the observation of shifts in terrestrial water storage (TWS) in reponse to climate and human activities. Robust detection and attribution of these changes remain a challenge because TWS exhibits strong seasonal variability and is traditionally observed at coarse spatial and temporal resolution. Recent studies have shown that direct regression of Level-1B observations (inter-satellite range data) from the Gravity Recovery and Climate Experiment (GRACE) and its Follow-On mission (GRACE-FO) can substantially improve effective spatial resolution of regression terms, compared to popular monthly mascon products. Applying this framework, we demonstrate that stacked Level-1B regression yields spatially refined estimates of both long-term TWS trends and seasonal amplitude, improving the ability to identify regions where human land and water use alter local freshwater availability. For trend analysis, the enhanced resolution strengthens attribution of storage change to anthropogenic drivers such as irrigation, groundwater extraction, reservoir operations, and land-use change at sub-basin scales. For seasonal characterization, we show that assuming simplified representations of the annual cycle, such as stationary, symmetric, or unimodal seasonality, can enable robust recovery of mean annual TWS amplitude with substantially reduced signal attenuation and leakage. Such refinements are particularly important for applications that depend on accurate annual water budgets, including water-balance-based evapotranspiration estimation and assessments of interannual hydroclimatic variability. The spatial scale at which GRACE satellites can independently observe water resources will continue to improve as additional years of measurements become available.

 

How to cite: O'Neill, M. M., Rodell, M., and Loomis, B.: Spatially refined global terrestrial water storage trends and annual cycles from GRACE and GRACE-FO, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16019, https://doi.org/10.5194/egusphere-egu26-16019, 2026.

EGU26-16439 | ECS | Orals | G3.1

Reconstructing terrestrial water storage anomalies based on climate data and pre-GRACE satellite observations 

Charlotte Hacker, Benjamin D. Gutknecht, Anno Löcher, and Jürgen Kusche

The Gravity Recovery And Climate Experiment (GRACE) and its follow-on mission, GRACE-FO, have observed global mass changes and transports, expressed as total water storage anomalies (TWSA), for over two decades. However, for climate change attribution and other applications, multi-decadal TWSA time series are required. This need has prompted several studies on reconstructing TWSA using regression or machine learning techniques, aided by predictor variables such as rainfall and sea surface temperature. However, the training period is limited to a couple of years, making it hard to capture interannual signals accurately. Furthermore, learned relationships between climate variables and water storage cannot be transferred straightforwardly to the past. To overcome the limitation and provide a more long-term, consistent dataset, we derive a preliminary reconstruction and combine it with large-scale time-variable pre-GRACE gravity information from geodetic satellite laser ranging (SLR) and Doppler Orbitography by Radiopositioning Integrated on Satellite (DORIS) tracking from Löcher et al. (2025). We reconstruct GRACE-like TWSA for the global land, excluding Greenland and Antarctica, from 1984 onward. We find that the seasonal cycle of our new reconstruction is consistent with that of previously published purely climate-data-based reconstructions. Moreover, in many regions, TWSA trends were markedly different in the pre-GRACE timeframe, and we thus suggest caution when interpolating GRACE-derived trends.

 

How to cite: Hacker, C., Gutknecht, B. D., Löcher, A., and Kusche, J.: Reconstructing terrestrial water storage anomalies based on climate data and pre-GRACE satellite observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16439, https://doi.org/10.5194/egusphere-egu26-16439, 2026.

In existing GNSS-based terrestrial water storage (TWS) inversion studies, the PREM model is commonly adopted, and crustal structural heterogeneity is often neglected. Here, we conduct a comprehensive assessment of how different Earth models affect inversion results using both checkerboard-model experiments and continuous smooth-model experiments. The results show that, under realistic hydrological loading conditions within the study region (100°E–115°E, 25°N–40°N), inversion differences among global 1-D reference Earth models are below 2%, whereas the differences between global 1-D reference models and regional crustal models are ~11%; meanwhile, discrepancies between the two regional crustal models remain below 4%. Application to observed GNSS coordinate time series in Yunnan indicates that the spatial pattern of the annual equivalent water height (EWH) amplitude derived from GNSS is broadly consistent with that from the GLDAS hydrological model; however, the choice of Earth model can still substantially alter the magnitude of the inferred amplitude and its spatial distribution. Correlation analyses further suggest that Earth-model dependence is weak for large-scale inversions, but becomes non-negligible at smaller spatial scales. For a representative small-scale subregion (101.75°E–102°E, 22.75°N–23°N), we therefore recommend using the AK135F model to construct Green’s functions. Overall, our findings demonstrate that Earth-model selection is a key source of uncertainty in GNSS-based TWS inversion, and provide practical guidance for choosing appropriate Earth models to improve inversion accuracy.

How to cite: He, J. and Li, Z.: Impact of Earth Model Selection on Terrestrial Water Storage Inversion from GNSS Vertical Displacements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17088, https://doi.org/10.5194/egusphere-egu26-17088, 2026.

EGU26-18067 | ECS | Orals | G3.1

Constraining transient solid Earth rheology using satellite orbit perturbations to assess the dynamics of climate change 

Maxime Rousselet, Alexandre Couhert, Kristel Chanard, Pierre Exertier, and Luce Fleitout

Monitoring essential climate variables such as Sea level rise, Earth’s Energy Imbalance, and ice-mass changes relies critically on space-geodetic observations of surface deformation and variations of the gravity field.
In particular, satellite geodesy provides decades-long, globally consistent records that are fundamental for quantifying climate-driven surface mass redistribution. However, these observations integrate both mass changes from the oceans, atmosphere, cryosphere and continental hydrology and the associated solid Earth response. Isolating climate variables from geodetic data therefore requires models that reflect the solid Earth response across timescales relevant to contemporary variability.
Yet, a critical assumption underlies much of current space-geodetic standard processing: the solid Earth response to surface mass variations is treated as purely elastic, i.e. instantaneous and fully recoverable. However, there is a growing body of evidence from laboratory rock mechanics experiments and geophysical observations suggesting that the Earth’s mantle exhibits a time-dependent, recoverable anelastic response across intermediate timescales  that could significantly affect geodetic at decadal to centennial timescales.
Here, we exploit several decades of Satellite Laser Ranging (SLR) observations towards passive spherical satellites to constrain key parameters governing the time-dependent mantle anelasticity. Owing to long-term measurements and sensitivity to low-degree gravity field variations, including solid Earth tides (C20, C30) and the pole tide (C21/S21), SLR observations are particularly well suited to probing deep Earth mantle rheology over decadal timescales.
We combine analytical orbit perturbation theory with the Hill-Clohessy-Wiltshire equations to quantify the sensitivity of the SLR observables to rheology and to choose an optimal parametrization. We then numerically estimate the solid Earth transient rheological properties from the SLR time series using an anelasticity framework consistent with seismic attenuation theory. Our results are compared with independent rheological constraints and yield a new set of frequency-dependent Love numbers that capture the Earth’s mantle transient rheology across decadal timescales.
We further show that accounting for this  transient rheology by incorporating the corresponding frequency-dependent Love numbers into the modeling of solid Earth tides, pole tide and surface loading-induced deformation, introduces systematic differences in climate-relevant geodetic time-series, including  satellite altimetry sea level rise estimates and ocean mass trends derived from satellite gravimetry.
More broadly, our results show that as space geodetic records become longer, data processing cannot rely solely on an  elastic solid Earth assumption. Instead, it must account for solid Earth transient rheology and the fact that geodetic observables will increasingly depend on the cumulative loading history, strengthening the need for interdisciplinary geodetic, geophysical and climate studies.

How to cite: Rousselet, M., Couhert, A., Chanard, K., Exertier, P., and Fleitout, L.: Constraining transient solid Earth rheology using satellite orbit perturbations to assess the dynamics of climate change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18067, https://doi.org/10.5194/egusphere-egu26-18067, 2026.

EGU26-18146 | ECS | Posters on site | G3.1

Uncertainties in Antarctic elevation change estimates by comparing radar and laser altimetry 

Maria T. Kappelsberger, Johan Nilsson, Martin Horwath, Veit Helm, Alex S. Gardner, and Matthias O. Willen

Since 1992, surface elevation change estimates of the Antarctic Ice Sheet (AIS) have been derived from satellite radar altimetry. However, large uncertainties remain due to local topography and the time-variable signal penetration into snow and firn. The unprecedented accuracy of measurements from the ICESat-2 satellite laser altimetry mission, launched in 2018, now enables inter-comparison with radar altimetry results. The primary goal of this study is to improve understanding of the uncertainties in AIS volume and mass balance estimates by quantifying how results from ICESat-2 and the CryoSat-2 radar altimetry mission diverge under different processing regimes. To do so, we analyse coincident ICESat-2 and CryoSat-2 measurements over the 6.9 million km² area of the relatively flat and large AIS interior, where topography-related errors are small. We apply a suite of state-of-the-art correction methods to the CryoSat-2 measurements, including multiple retracking algorithms and empirical corrections for the time-variable surface and volume scattering of the radar signal. From April 2019 to October 2024, ICESat-2 observations show a thickening of 97 ± 4 km3 yr−1, coincident with excess snowfall in this period. CryoSat-2 solutions indicate systematically lower thickening rates than ICESat-2. The smallest bias (0.6 ± 1.0 cm yr−1 or 42 km3 yr−1) between the results from the two missions is found when using the AWI-ICENet1 convolutional neural network retracker. One of our hypotheses is that the systematic radar-laser differences might be due to residual errors related to the time-variable radar penetration, particularly affected by the heavy snowfall events in recent years. While further work is needed to test this hypothesis, our study demonstrates both the challenges of resolving subtle, long-term surface mass balance trends using radar altimetry and the value of joint laser-radar analyses for improving AIS volume and mass balance estimates.

How to cite: Kappelsberger, M. T., Nilsson, J., Horwath, M., Helm, V., Gardner, A. S., and Willen, M. O.: Uncertainties in Antarctic elevation change estimates by comparing radar and laser altimetry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18146, https://doi.org/10.5194/egusphere-egu26-18146, 2026.

EGU26-18337 | ECS | Orals | G3.1

Impact of NGGM and MAGIC on Sea Level and Energy Budgets Closure 

Ramiro Ferrari, Julia Pfeffer, Marie Bouih, Benoît Meyssignac, Alejandro Blazquez, and Ilias Daras

The SING project aims to evaluate the added value of the NGGM and MAGIC missions for scientific applications and operational services in hydrology, ocean sciences, glaciology, climate sciences, solid earth sciences, and geodesy. Using a closed-loop simulator with a comprehensive description of instrumental, ocean tide, dealiasing and toning errors, synthetic observations of the gravity field have been generated to assess the observability of mass changes occurring in the atmosphere, ocean, hydrosphere, cryosphere, and solid earth for different mission configurations, including GRACE-C-like (single polar pair), NGGM (single inclined pair), and MAGIC (double pair). 

The synthetic gravity observations have first been used to assess the closure of the sea level budget. With historical GRACE, altimetry, and Argo data, global sea level budget closure is achieved with an accuracy of 0.3–0.4 mm/yr (2003–2015). Using VADER-filtered simulations, all three configurations contribute <0.1 mm/yr to the global mean sea level error. NGGM and MAGIC maintain this accuracy even without filtering, unlike GRACE-C. At regional scales, NGGM and MAGIC notably improve significantly the sea level budget closure, especially at seasonal and interannual timescales, though gains for decadal trends remain modest. 

The synthetic gravity observations were also used to assess the closure of the global energy budget. Historical gravimetry, altimetry, and Argo data yield global mean ocean heat uptake (GOHU) accuracy of 0.2–0.3 W/m² (2003-2015). With VADER-filtered simulations, GRACE-C-like missions contribute up to 0.19 W/m² uncertainty, while NGGM and MAGIC improve this by 30–40%, achieving ~0.12–0.13 W/m² accuracy. They also enhance the stability and temporal consistency of GOHU retrievals. Regionally, NGGM and MAGIC outperform GRACE-C by up to 80% in recovering ocean heat content changes at mid-latitudes (30–60° N/S). Slightly better results are obtained with NGGM due to the use of mission error covariance information in the VADER filter. NGGM and MAGIC recover mean and temporal variations in ocean heat uptake at regional scales with up to 50% higher accuracy than GRACE-C.
The NGGM and MAGIC missions will substantially enhance the accuracy, spatial and temporal resolution of gravity-based observations of sea level changes and its drivers. These improvements strengthen global climate assessments, support the evaluation of mitigation policies, and improve climate model validation. In particular, sustained and redundant monitoring of ocean heat uptake would provide an early and robust indicator of changes in radiative forcing, preceding detectable stabilization of global temperatures by several decades. Improved characterization of regional heat-uptake pathways also enhances projections of sea level rise, marine heat extremes, and ocean circulation changes, supporting climate risk management across coastal, marine, and ecosystem applications.

How to cite: Ferrari, R., Pfeffer, J., Bouih, M., Meyssignac, B., Blazquez, A., and Daras, I.: Impact of NGGM and MAGIC on Sea Level and Energy Budgets Closure, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18337, https://doi.org/10.5194/egusphere-egu26-18337, 2026.

EGU26-18774 | Posters on site | G3.1

How is the global and regional sea level budget closed from the latest observations?  

Marie Bouih, Robin Fraudeau, Julia Pfeffer, Ramiro Ferrari, Michaël Ablain, Anny Cazenave, Benoît Meyssignac, Alejandro Blazquez, Martin Horwath, Jonathan Bamber, Antonio Bonaduce, Roshin Raj, Stéphanie Leroux, Nicolas Kolodziejczyk, William Llovel, Giorgio Spada, Andrea Storto, Chunxue Yang, and Erwan Oulhen and the ESA SLBC CCI+ team

The closure of the Sea Level Budget (SLB) is a key challenge for modern physical oceanography. First, it is essential that we ensure the proper identification and quantification of each significant contributor to sea level change through this closure. Second, it provides an efficient means to closely monitor and cross-validate the performance of intricate global observation systems, such as the satellite altimetry constellation, satellite gravimetry missions (GRACE/GRACE-FO), and the Argo in-situ network. Third, this closure reveals to be a beneficial approach for assessing how well the observed climate variables, such as sea level, barystatic sea level, temperature and salinity, land ice melt, and changes in land water storage, comply with conservation laws, in particular those related to mass and energy.

In this presentation, we will discuss the state of knowledge of global mean and regional sea level budget with up-to-date observations, encompassing 1) an up-to-date assessment of the budget components and residuals, along with their corresponding uncertainties, spanning from 1993 to 2023 in global mean and throughout the GRACE and Argo era for spatial variations; 2) the identification of the periods and areas where the budget is not closed, i.e. where the residuals are significant; 3) advancements in the analysis and understanding of the spatial patterns of the budget residuals. 

To investigate the sea level budget (SLB) misclosure, we developed an objective solution that closes the SLB globally. This approach is based on an inverse method that optimally combines the contributions to sea level, weighted by their estimated instrumental uncertainties, and draws from publications such as those by Rodell et al. (2015) and L’Ecuyer et al. (2015).

This objective method allows us to precisely identify the dates when the SLB misclosure falls outside the uncertainty estimates, as well as the contributor most likely responsible for the discrepancy. The results of this analysis will be detailed during the presentation.

A focus will be made on the North Atlantic Ocean where the residuals are significantly high. We investigate the potential errors causing non-closure in each of the components (e.g., in situ data sampling for the thermosteric component, geocenter correction in the gravimetric data processing) as well as potential inconsistencies in their processing that may impact large-scale patterns (e.g., centre of reference and atmosphere corrections). 

This work is performed within the framework of the Sea Level Budget Closure Climate Change Initiative (SLBC_cci+) programme of the European Space Agency (https://climate.esa.int/en/projects/sea-level-budget-closure/). This project was initiated by the International Space Science Institute Workshop on Integrative Study of Sea Level Budget (https://www.issibern.ch/workshops/sealevelbudget/).

How to cite: Bouih, M., Fraudeau, R., Pfeffer, J., Ferrari, R., Ablain, M., Cazenave, A., Meyssignac, B., Blazquez, A., Horwath, M., Bamber, J., Bonaduce, A., Raj, R., Leroux, S., Kolodziejczyk, N., Llovel, W., Spada, G., Storto, A., Yang, C., and Oulhen, E. and the ESA SLBC CCI+ team: How is the global and regional sea level budget closed from the latest observations? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18774, https://doi.org/10.5194/egusphere-egu26-18774, 2026.

EGU26-75 | Posters on site | HS1.1.2

A Low-Cost Flood-Proof Water Level Measurement System, Using GNSS Reflectrometry 

Nick van de Giesen, Tijs De Laere, Jort van Driel, Ward van der Bijl, and Stefan Loen

Global Navigation Satellite System Interferometric Reflectometry (GNSS-IR) is a well-established technology to determine water heights in reservoirs, rivers, and lakes. A big advantage of GNSS-IR over traditional level measurements is that it is a non-contact flood-proof method. So far, GNSS-IR has been applied through off-site processing, necessitating a good internet connection for near-real-time monitoring. In Africa, where the TEMBO project seeks to develop in situ monitoring of weather and water, such connections are often not available, especially in more remote river valleys. Although a live satellite uplink would be possible, these tend to be costly and very energy-hungry. For this reason, equipment was developed that allowed local processing (edge processing). The advantage is that only water levels and some system information need to be communicated, which can be done with a simple satellite modem at very moderate costs. Existing gnssrefl code (https://gnssrefl.readthedocs.io/), written in Python, was rewritten in Rust to facilitate running the code on a PICO 2.  By reducing unneeded lines of code, the runtime was reduced from three minutes with the original Python code to less than three seconds. In all, energy use was minimized to avoid the need for large solar panels. With power cycling and uploads four times per day, the average power consumption was 44mW, which translates into a small solar panel of 1.2 W (66mm x 113mm). Water level measurement accuracy depended on integration time or, better, the number of satellites captured and was about 8cm when five or more satellites were captured. Total material costs, excluding the satellite modem, were about EU 50. The satellite modem and antenna were, at EU 360, the most expensive parts.

TEMBO Africa: The work leading to these results has received funding from the European Horizon Europe Programme (2021-2027) under grant agreement n° 101086209. The opinions expressed in the document are of the authors only and in no way reflect the European Commission’s opinions. The European Union is not liable for any use that may be made of the information.

How to cite: van de Giesen, N., De Laere, T., van Driel, J., van der Bijl, W., and Loen, S.: A Low-Cost Flood-Proof Water Level Measurement System, Using GNSS Reflectrometry, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-75, https://doi.org/10.5194/egusphere-egu26-75, 2026.

EGU26-1566 | ECS | Posters on site | HS1.1.2

Acoustic Sensor–Based Borehole Monitoring in Semi-Arid African Regions 

Anna Geofrey, Rolf Hut, and Nick van de Giesen

Wells and boreholes have long served as critical sources of freshwater in the semi-arid and arid regions of Africa. Despite their importance, effective monitoring of these water points remains limited due to the high cost of establishing and maintaining dedicated observation wells, resulting in sparse and unreliable datasets. This study explores a cost-effective approach to groundwater monitoring by equipping operational wells and boreholes with low frequency acoustic sensors integrated into a scalable wireless sensor network. The system enables continuous acquisition of time-series data on water levels, discharge rates, and recharge dynamics. The major innovation here is that we use existing and operational water infrastructure as monitoring points. The presentation will demonstrate the principles, advantages, and obstacles that still need to be overcome. The proposed method improves data availability and supports more sustainable groundwater management across data-scarce regions in Africa.

How to cite: Geofrey, A., Hut, R., and van de Giesen, N.: Acoustic Sensor–Based Borehole Monitoring in Semi-Arid African Regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1566, https://doi.org/10.5194/egusphere-egu26-1566, 2026.

Measuring open-channel hydraulics is crucial, for example, for deriving discharges from stage observations, estimating travel times for pollutant plumes, and assessing riverbed dynamics. State-of-the-art surveying approaches are typically conducted along predefined cross-sections of the river course, either manually using a flow meter or with instrumented boats. The latter are technologically advanced platforms equipped with electric propulsion, ADCP sensors, and high-precision RTK-GPS and may cost several tens of thousands of US dollars (or euros). To fill data gaps between cross-sections, surveys often rely on longitudinal boat campaigns, which are generally feasible only in larger streams without hydraulic barriers.

To support water authorities with limited budgets, particularly to survey smaller streams, we developed MONIKA, a low-cost surveying catamaran. In accordance with its acronym, MONIKA is comprised of three primary functions: MO - Monitoring (continuous tracking of water parameters), NI - Navigation (movement along and across the stream), and KA -  Kartography (mapping of the riverbed morphology). The platform is equipped with a castable sonar, GPS, and two CTD (Conductivity-Temperature-Depth) dataloggers. As an additional payload, a commercial high-precision inclination sensor is deployed to monitor the water surface slope. All data-processing steps are implemented in an object-oriented framework within an open-source Python package.

After extensive testing and design optimization, the engine-less boat can be deployed in two operational modes: (1) bank-guided operation using an aluminum rod and snap hook, and (2) free-floating operation in which the boat is retrieved with a net installed at the downstream end of the study reach. The free-floating mode is particularly suited for surveying riverbed slope, as it avoids operator-induced interference with inclination measurements.

As an initial application, MONIKA, was deployed at two sections of the Spree River (Germany) to support the placement of new sampling stations downstream of a river confluence. MONIKA was used to determine the minimum downstream distance required for complete mixing. Future applications will extend this approach to open-channel surveys in small rivers, with a particular emphasis on data-scarce catchments.

How to cite: Nixdorf, E., Böhmeke, M., and Gatzke, F.: Development of a low-cost water vehicle for surveying river bed elevation and chemo-physical changes along the river course , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4963, https://doi.org/10.5194/egusphere-egu26-4963, 2026.

EGU26-5086 | Posters on site | HS1.1.2

A cost-effective rock sample unit for quality control and intercomparison of 222Rn measurements 

Frédéric Huneau, Sebastian Grondona, Sébastien Santoni, Seng Chee Poh, Tibari El Ghali, Stefan Terzer-Wassmuth, and Mélanie Vital

Reliable radon-222 measurements are essential for a wide range of hydrological, geological, and environmental applications, including the study of surface water - groundwater interactions and the quantification of groundwater discharge. Despite the widespread use of 222Rn detectors, routine verification of instrument performance and measurement stability remains limited, particularly in laboratories with constrained financial and technical resources. This study presents the development and evaluation of a cost-effective rock sample unit designed to support quality control, calibration checks, and inter-laboratory comparison of 222Rn measurements.

The system is based on acidic plutonic igneous rock purchased from commercial suppliers, selected for their naturally elevated and stable 222Rn production. The rocks were enclosed in a simple, airtight container assembled using readily available components, including a standard garden filter and plastic tubing. This configuration allows 222Rn generated within the rock matrix to accumulate in a closed volume and be circulated through commonly used 222Rn detectors without the need for specialized or commercial equipment. Equal amounts of material were placed in each rock sample unit, which were then sealed and stored for 21 days to allow 222Rn to reach secular equilibrium with its parent radionuclides. Initial characterization of the rock units was performed at the IAEA Isotope Hydrology laboratory. Each unit was analysed three times using a standardized protocol consisting of six measurement cycles of 30 minutes each. Measurements were conducted using RAD7 and RAD8 222Rn detectors from Durridge, which are widely applied in environmental and hydrological studies. The results demonstrated stable and reproducible 222Rn concentrations across repeated measurements, confirming the suitability of the rock units as reference sources for quality control purposes.

Following this initial validation, the previously measured rock sample units were distributed to participating laboratories in Argentina, France, Malaysia, and Morocco. Each laboratory applied the same measurement protocol and used their routinely operated 222Rn detectors (RAD7 and RAD8).

To support the interpretation of the observed variability, contextual information was considered, including the age of the instrument, the date of last recalibration, the intensity of use, the type of water typically analysed (saline or non-saline; surface water or groundwater), and the range of 222Rn concentrations normally encountered. This approach enabled the assessment of the significance of deviations under different operating conditions and allowed the evaluation of the robustness of measurements obtained with calibrated versus non-calibrated instruments.

This exercise showed that even simple comparison of 222Rn responses obtained from the rock units provides valuable insight into the performance of the instrument and detect the potential measurement drift related to the lack of calibration. The results demonstrate that these cost-effective rock sample units represent a practical and accessible tool for strengthening 222Rn measurement quality assurance. Their simplicity, low resource requirements, and reproducibility make them particularly suitable for routine checks, contributing to the improved comparability of 222Rn data.

How to cite: Huneau, F., Grondona, S., Santoni, S., Poh, S. C., El Ghali, T., Terzer-Wassmuth, S., and Vital, M.: A cost-effective rock sample unit for quality control and intercomparison of 222Rn measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5086, https://doi.org/10.5194/egusphere-egu26-5086, 2026.

EGU26-11522 | Posters on site | HS1.1.2

Automated sampling of dew water to identify hidden nutrient inputs to ecosystems 

Jannis Groh, Andreas Lücke, Thomas Pütz, Ferdinand Engels, Roger Funk, Andreas Sitnikow, Daniel Beysens, and Wulf Amelung

The terrestrial water and nutrient cycle is of crucial importance, influencing the climate, ecosystems, and related services. In many climates, non-rainfall water inputs (NRWIs) play a significant role in the water cycle. These inputs stem from various processes, including dew, fog, and soil water vapour adsorption. Weighable lysimeters are ideal tools for quantifying such water inputs to ecosystems, as their surfaces are either plant- or soil-covered, which is relevant for their formation processes, compared to devices with artificial surfaces. However, the nutrient inputs from dew and fog, apart from wet and dry deposition, are yet to be overlooked, as it is difficult to monitor these hidden nutrient inputs to ecosystems without adequate sampling devices.

We present a newly developed dew collector for the regular collection and analysis of dew samples, for example for stable isotopes, nutrients, and other substances. The lack of automated methods for collecting dew samples represents a significant bottleneck to account for these hidden nutrient inputs. Using a comprehensive measurement setup with weighable lysimeters, wet and dry deposition, and dew and fog water collectors, we show how NRWIs introduce nutrients into ecosystems with different land uses (grassland and cropland) in a temperate climate.

How to cite: Groh, J., Lücke, A., Pütz, T., Engels, F., Funk, R., Sitnikow, A., Beysens, D., and Amelung, W.: Automated sampling of dew water to identify hidden nutrient inputs to ecosystems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11522, https://doi.org/10.5194/egusphere-egu26-11522, 2026.

EGU26-12528 | Posters on site | HS1.1.2

Low-cost spectrophotometer for measuring nitrogen dioxide (NO2) air pollution 

Bas Mijling and Rolf Hut

Palmes diffusion tubes are widely used as a low-cost method for measuring ambient nitrogen dioxide (NO2) air pollution. Based on the principle of molecular diffusion, ambient NO2 accumulates as nitrite at the closed end of the tube. After a typical four-week exposure period, the tubes are returned to a laboratory, where the nitrite is dissolved in water, reacted with a colorimetric reagent, and quantified by measuring the resulting color change using a spectrophotometer.

Despite their effectiveness and affordability, Palmes diffusion tubes are still rarely used in Africa. A major reason is that tube preparation and analysis are typically must be carried out in laboratories outside the continent. One key barrier to establishing local Palmes laboratories is the high upfront cost of spectrophotometers required for sample analysis.

While conventional spectrophotometers can measure absorbance across a wide range of wavelengths, most reagent-based colorimetric analyses require only a single wavelength. For Palmes tube analysis, absorbance is measured at 540 nm, corresponding to the maximum absorption of the Griess reagent. Since green LEDs emit light within a narrow waveband close to this absorption peak, they offer a low-cost alternative light source.

We present and will live-demonstrate a simple device that replaces the spectrophotometer in the Palmes tube analysis workflow. The device consists of a 3D-printed light-tight cuvette holder housing a green LED for illumination and a photodiode to measure transmitted light. Measurement results are displayed directly on the device. The system can determine nitrite concentrations with an accuracy of 3 µg/L, corresponding to approximately 0.1 µg/m3 of ambient NO2 for a four-week exposure period—well below the intrinsic uncertainty of the Palmes diffusion method.

Costing only a fraction of a conventional spectrophotometer, this device has the potential to greatly expand in-situ monitoring of NO2 pollution in sub-Saharan Africa without substantially increasing costs. Moreover, it provides a promising proof of concept for developing similar low-cost instruments for other air and water quality applications based on colorimetric measurements.

How to cite: Mijling, B. and Hut, R.: Low-cost spectrophotometer for measuring nitrogen dioxide (NO2) air pollution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12528, https://doi.org/10.5194/egusphere-egu26-12528, 2026.

EGU26-16212 | Posters on site | HS1.1.2

A novel geophysical electric field sensor design and testing 

Da Lei and Qihui Zhen

One of the Earth's natural physical fields is the geoelectric field. The conductivity of subterranean medium and the locations of pollution sources, among other things, may be examined by tracking variations in the geoelectric field signal over time. The success rate of resource exploration and the accuracy of geological structure inversion are closely correlated with signal quality. Conventional geoelectric field measurement techniques use electrochemical non-polarizing electrodes to detect the potential difference between two electrodes that are far apart in order to acquire the geoelectric field signal. The potential difference value that exists between the electrodes for their own causes is called the "range difference."  Environmental conditions will influence the electrodes' range difference, and the range difference variation amplitude will be greater than the amplitude of the actual geoelectric field signal. Non-polarizing electrodes must be buried deep below during the actual measuring procedure, and electrolyte solutions must be poured to lower the grounding impedance. The electrolyte solution is prone to evaporation or loss in unique environments like deserts and the Gobi, which might result in an abrupt rise in the grounding impedance of the non-polarizing electrodes. This will impact the precision of the geoelectric field signal measurement findings.

This design, which is based on the charge induction principle, aims to create a new kind of electric field sensor that can continuously measure the geoelectric field signal without range differences and does not require the electrodes to be buried. The viability of this sensor is confirmed using physical models and circuit simulations, as well as by contrasting the geoelectric field signal measurement findings of the physical product with those of solid non-polarizing electrodes.

How to cite: Lei, D. and Zhen, Q.: A novel geophysical electric field sensor design and testing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16212, https://doi.org/10.5194/egusphere-egu26-16212, 2026.

EGU26-18536 | Posters on site | HS1.1.2

Analysis of Nitrate Stable Isotopes by Cavity Ring-Down Spectroscopy 

Jennifer McKay, Cedric Douence, Magdalena Hofmann, Jan Woźniak, and Joyeeta Bhattacharya

Nitrate contamination of surface and groundwater is a serious environmental and public health issue.  Identifying the source of this pollutant is an important step in addressing the problem. Nitrogen and oxygen isotopes (δ15N and δ18O values) are a powerful tool for tracing the source(s) of nitrate and understanding processes that impact its cycling in the environment.  Traditionally nitrate isotopes are measured via isotope ratio mass spectrometry (IRMS) but in recent years laser spectroscopy has become a practical option.

We evaluated Picarro’s new PI5131-i isotopic and gas concentration analyser for determining bulk δ15N and δ18O values of N2O converted from dissolved nitrate using the Titanium III chloride method. The PI5131-i analyser is based on a robust mid-infrared, laser-based cavity ring-down spectrometry (CRDS) technology. This system when combined with Picarro’s Sage gas autosampler allowed us to analyse the isotopic composition of dissolved nitrate to a level matching IRMS precision and at concentrations as low as 0.05 mg/L NO3-N. 

In 40 mL reaction vials, Ti (III) chloride was added to 10 mL sample at a 1:20 ratio (v/v, reagent to sample). After 24 hours of reaction time enough N2O was produced for laser spectroscopy analysis. Prior to analysis, the headspace N2O was transferred into 12 mL exetainers to fit in the Sage autosampler. We compared a direct transfer protocol where 2 mL N2O from the reaction vial is injected into exetainers and a 2-steps protocol where the N2O is injected into purged exetainers (evacuated and pressurized with synthetic air).

Both transfer methods performed well in a blind nitrate intercomparison exercise (NICO).  The direct transfer workflow required fewer preparation steps but required a blank correction, whereas the two-step protocol was more labour-intensive due to the purge and fill process.

How to cite: McKay, J., Douence, C., Hofmann, M., Woźniak, J., and Bhattacharya, J.: Analysis of Nitrate Stable Isotopes by Cavity Ring-Down Spectroscopy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18536, https://doi.org/10.5194/egusphere-egu26-18536, 2026.

EGU26-19260 | ECS | Posters on site | HS1.1.2

EVE: a low-cost, modular, end-to-end monitoring pipeline for environmental variables and GHG in rewetted peatlands 

Milan Shay Kretzschmar, Maren Dubbert, Matthias Lück, Michael Asante, Geoffroy Sossa, and Mathias Hoffmann

Rewetted peatlands exhibit strong small-scale, spatio-temporal variability in their greenhouse gas (GHG; CO₂, CH₄ and N₂O) emissions. Those are shaped by water table dynamics, vegetation structure, and microclimate. Capturing “hotspots” and “hot moments” across heterogeneous peatlands typically requires dense instrumentation. However, conventional monitoring solutions remain expensive, difficult to scale, and often depend on commercial, vendor-locked systems. We present the Environmental Variables Explorer (EVE) as a low-cost, modular, open-source alternative that enables researchers to build, repair, adapt, and self-host their monitoring stack without vendor lock-in.

EVE is a platform blueprint rather than a single device. It combines low-power microcontroller nodes with power-saving duty cycling and two interoperable end-to-end, full user controlled workflows. The first, offline workflow, provides robust timestamped local storage (RTC + FRAM) with Bluetooth retrieval via a custom Android app - suited for remote sites. The second, online workflow, uses an ESP32 IoT node to upload measurements via Wi-Fi to a self-hosted PHP/MySQL backend that provides a web dashboard, API access, data visualization and data export (as CSV file) on inexpensive shared hosting. Critically, the offline-online duality provides a “fallback” logic for intermittently connected peatland environments and supports gradual scaling from single devices to multi-site networks.

Building on EVE’s user-controlled pipeline, we present a pathway toward transferable near-real-time analytics by adding chamber-based GHG modules (low-cost CO₂/CH₄ sensing and chamber automation/sampling workflows. Integrating data-driven models (Random Forest and related methods) to estimate flux dynamics and annual budgets across 2-3 sites. Explicitly comparing high-end versus minimal low-cost inputs. By releasing hardware designs, firmware, backend code, and build documentation, this work aims to lower barriers for peatland and other scientists to deploy reproducible monitoring networks and to move toward shared, community-driven approaches for scalable GHG observation and modeling.

How to cite: Kretzschmar, M. S., Dubbert, M., Lück, M., Asante, M., Sossa, G., and Hoffmann, M.: EVE: a low-cost, modular, end-to-end monitoring pipeline for environmental variables and GHG in rewetted peatlands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19260, https://doi.org/10.5194/egusphere-egu26-19260, 2026.

EGU26-21344 | Posters on site | HS1.1.2

Low-Cost Water Quality Buoys: Open-Source Design and AI-Enhanced Monitoring  

Tom Rowan, Joaquina Noriega Gimenez, Yixuan Jia, Yanchi Tang, Ben Howard, Liam Kelleher, Luke Tumelty, Aaron Packman, Athanasios Paschalis, Stefan Krause, and Wouter Buytaert

Water quality monitoring networks face an inherent trade-off between measurement precision and spatial-temporal coverage. We present an open-source smart water quality buoy designed to explore the potential of maximising deployment density and sampling frequency through low-cost instrumentation combined with AI-enhanced analytics. 

The stable buoy enclosure was developed using computational fluid dynamics, water flume validation, and extensive field testing. Initially designed for 3D-printing, it houses three sensors (temperature, turbidity and conductivity) with an ATmega328P microcontroller, real-time clock, flash logging, and/or LoRaWAN connectivity. Laboratory calibration established measurement reliability suitable for network-scale deployment. 

Field deployments have demonstrated autonomous operation with a relatively light monthly maintenance protocol. This platform enables novel monitoring approaches that leverage density over individual sensor accuracy. Initial Machine Learning models trained on national databases (millions of observations) convert basic sensor measurements into estimates of complex parameters — nutrients, dissolved oxygen, and bacteria — with encouraging accuracy. The high-frequency data from dense sensor networks enables automated pollution detection by analyzing concentration dynamics and comparing them against patterns learned from a large database of water quality measurements.

By combining accessible hardware with AI analytics, we investigate whether prioritising spatial-temporal resolution can advance water quality monitoring capabilities, particularly for early pollution detection and regulatory compliance in under-resourced catchments. 

How to cite: Rowan, T., Noriega Gimenez, J., Jia, Y., Tang, Y., Howard, B., Kelleher, L., Tumelty, L., Packman, A., Paschalis, A., Krause, S., and Buytaert, W.: Low-Cost Water Quality Buoys: Open-Source Design and AI-Enhanced Monitoring , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21344, https://doi.org/10.5194/egusphere-egu26-21344, 2026.

The emergence of Unmanned Aerial Systems (UAS) has revolutionized environmental monitoring by bridging the gap between stationary ground-based stations and coarse-resolution satellite imagery. However, integrating high-fidelity sensors into lightweight platforms remains a challenge due to strict Size, Weight, and Power (SWaP) constraints. This study presents the development and deployment of an advanced, portable sensing payload designed for high-resolution environmental data collection.

The integrated payload consists of a suite of low-cost yet calibrated sensors capable of measuring Isme PM2.5, CO2, NH4, Smoke and O3 at high temporal frequencies. To ensure data integrity, the system incorporates an onboard microprocessor for real-time data fusion, GPS-tagging, and active aspiration systems to mitigate the effects of rotor wash and thermal interference.

Preliminary field campaigns were conducted across two locations (Dehradun, Uttarakhand and New Delhi) to evaluate the system’s performance. Results indicate that the payload provides vertical and horizontal spatial resolutions previously unattainable with traditional methods. This work highlights the potential of modular UAS payloads to provide actionable insights into boundary layer dynamics and pollutant dispersion in complex terrains.

To ensure data integrity, the platform integrates active aspiration systems designed to decouple sensor readings from the effects of rotor wash and localized thermal artifacts. Initial experiments demonstrate that the payload achieves high-granularity in vertical and horizontal spatial resolutions.

How to cite: Natoo, A.: Developing a Lightweight UAS sensing Payload for Environmental Data collection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21545, https://doi.org/10.5194/egusphere-egu26-21545, 2026.

EGU26-23048 | Posters on site | HS1.1.2

In a Grassed Waterway the grass is always greener – and surface runoff a challenge to measure 

Matthias Konzett, Peter Strauss, Christopher Thoma, Dušan Marjanovic, Borbala Szeles, Günter Blöschl, and Elmar Schmaltz

Grassed waterways (GWW) are a nature-based solution in agricultural catchments to reduce surface runoff and soil erosion. However, continuous measurements of surface runoff in a GWW remain challenging, limiting knowledge of how to construct a measurement station to obtain reliable data. Furthermore, these limitations restrict our understanding of hydrological processes and the effectiveness of GWWs. In this study, we present a monitoring station designed to measure surface runoff and quantify soil erosion from a 6 ha agricultural sub-catchment, and discuss the opportunities and limitations of monitoring runoff, sediments, and nutrients in a managed GWW. This study is part of the overall 66 ha catchment at the HOAL (Hydrological Open-Air Laboratory), Austria.  

We developed an H-Flume-like structure that reliably quantifies flow without disturbing the GWW’s function. Non-contact radar probes measure the height and velocity of runoff in the structure, allowing discharge calculations during runoff events. When a specified runoff height is detected, an automatic water sampler collects water for further analysis, such as sediment quantification. Thermal and optical cameras are mounted on the structure to capture images from upslope, the structure itself, and downslope, providing several perspectives for visual documentation of runoff processes and sediment transport.

While complementary measurements and modelling support the understanding of the overall effectiveness of the GWW in the HOAL catchment, this station provides valuable information on the timing of runoff, peak flow reduction, and catchment connectivity. The integrated sensor network at this station and throughout the HOAL - including rain gauges, soil moisture sensors, and additional runoff stations - enables a process-based understanding of how grassed waterways affect surface runoff, pluvial floods, and sediment and nutrient transport towards the stream.

This methodology remains under active development, and we encourage community input on improvements to the current methodologies and suggestions for additional observations. This presentation aims to share our current design, present preliminary results, and foster collaborative discussion on advancing monitoring of vegetated, nature-based erosion control structures.

How to cite: Konzett, M., Strauss, P., Thoma, C., Marjanovic, D., Szeles, B., Blöschl, G., and Schmaltz, E.: In a Grassed Waterway the grass is always greener – and surface runoff a challenge to measure, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23048, https://doi.org/10.5194/egusphere-egu26-23048, 2026.

EGU26-23272 | Posters on site | HS1.1.2

SMARTWATER: low-cost, open-source portable water autosampler for environmental monitoring 

Liam Kelleher and Kieran Khamis and the SMARTWATER Team

Water sampling is essential for assessing the quality of rural and urban water systems. As part of the NERC-NSFGEO SMARTWATER project we aim to diagnose pollution “hot spots” and “hot moments” within watersheds defined as locations and times of pollution transport. To understand and diagnose pollutant dynamics we are forming a smart monitoring network consisting of offline and online sensors, low-cost proxy sensor measurements, and event-based sample collection using autosamplers.

To address existing autosampler constraints, we have developed a smart online autosampler that can be triggered either by a float switch or remotely through a LoRa network. The system is optimised for low-power operation using 12V electronics, light and smaller lithium-based batteries, power optimised Arduino controller, LoRa shield, commercial solenoid values and relays. Laboratory testing has validated the system operation and effective flushing of water between sampling bottle fills. Field deployment along our urban observatory, the Birmingham Urban River Observatory, a UNESCO Intergovernmental Hydrological Programme site, demonstrated performance comparable to standard systems.

This open-source design enables scalable, cost-effective monitoring of river water quality, facilitating improved spatial and temporal assessment across multiple catchments. SMARTWATER: https://www.smart-water.org.uk/

How to cite: Kelleher, L. and Khamis, K. and the SMARTWATER Team: SMARTWATER: low-cost, open-source portable water autosampler for environmental monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23272, https://doi.org/10.5194/egusphere-egu26-23272, 2026.

CR7 – The Cryosphere in the Earth system: interdisciplinary topics

The Yarlung Zsangbo Grand Canyon (YGC) acts as a critical water vapor channel for the Tibetan Plateau, profoundly influencing regional and downstream hydrometeorology. Significant research progress has recently been made in understanding the complex precipitation processes within this unique corridor, integrating multi-source observations, satellite retrieval evaluation, and model simulations.

A core finding is the systematic underestimation of precipitation over the eastern Himalayas by widely used products like GPM IMERG, which has been quantitatively reduced through improved algorithms informed by dense in-situ gauge data. Comprehensive investigations utilizing a novel multi-platform observational network have elucidated the complete three-dimensional structure and life cycle of precipitation systems within the YGC. This network, combining ground-based radars, disdrometers, and radiosondes, has revealed distinct seasonal shifts in precipitation microphysics. Notably, mixed-phase and ice-phase processes play a key role in these seasonal transitions, with significant differences identified between the southeastern Tibetan Plateau and lower-altitude regions. Furthermore, two dominant types of heavy precipitation events have been classified and their distinct dynamic and thermodynamic mechanisms have been established.

Research also highlights the challenges of reanalysis accuracy in complex terrain, while providing pathways for improvement. Leveraging these mechanistic insights, recent efforts have successfully improved the forecasting of heavy precipitation in the YGC through optimized model physics, specifically by integrating enhanced cumulus and turbulent orographic form drag (TOFD) parameterization schemes. Collectively, these studies advance the quantitative understanding of precipitation processes in this major water vapor channel, offering crucial insights for hydrological modeling, climate studies, and numerical weather prediction in high-altitude complex terrain.

How to cite: Chen, X.: Research progress of precipitation process in the water vapor channel of Yarlung Zsangbo Grand Canyon, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1414, https://doi.org/10.5194/egusphere-egu26-1414, 2026.

EGU26-2245 | Posters on site | AS1.23

Kilometer-Scale Convection-Permitting Simulations in Representing Winter Precipitation over the Indian Himalayas 

Raju Attada, Nischal Sharma, Kieran Hunt, and Valentine Anantharaj

Kilometer-scale (k-scale) simulations, with explicit treatment of convection at sub-grid scales, are useful for understanding precipitation characteristics. Such simulations with their high spatiotemporal resolution can be particularly valuable in complex topographies like the Hindu Kush Himalayas (HKH), where sparse observations and uncertainties in coarse-resolution datasets pose challenges. This study evaluates a regional AMIP-style k-scale (1 km) simulation, initialised from the ECMWF IFS analysis, for winter mean and extreme precipitation (December 2018-February 2019) in the HKH region, using high-resolution gridded precipitation datasets from multiple sources. The model realistically depicts the spatial distribution of precipitation, particularly the ridge-valley variations, often missed in coarser products. In general, it aligns more with reanalysis datasets but closely matches station observations too. Mean precipitation exhibits sensitivity to elevation, and the highest rates occur at about 2500 m in most of the reference products (observations/reanalysis), which the k-scale model represents well. The diurnal cycle depicts sub-daily precipitation maxima in the local afternoon and early morning hours. The analysis for precipitation extremes indicates the model’s close fidelity with reanalysis products in capturing higher-intensity and prolonged precipitation events in the western Himalayas. Radiosonde profiles and atmospheric thermodynamic characteristics highlight a highly saturated and unstable environment during extremes, which is favourable for enhanced convective developments and heavy precipitation. The model captures these atmospheric conditions well and represents the localized variations and intensifications in valley wind flows during extremes, which are often missed in coarser-resolution and parameterized ERA5 data. Our findings highlight the added value of k-scale convection-permitting models over coarser-resolution, parameterized models in resolving subgrid-scale processes, particularly in complex terrains like the HKH, without the need for convective parameterization.

How to cite: Attada, R., Sharma, N., Hunt, K., and Anantharaj, V.: Kilometer-Scale Convection-Permitting Simulations in Representing Winter Precipitation over the Indian Himalayas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2245, https://doi.org/10.5194/egusphere-egu26-2245, 2026.

EGU26-3384 | ECS | Posters on site | AS1.23

Systematic analysis of flow-orography interactionin idealized numerical simulations 

Šimon Bartoň and Petr Šácha

Current generation climate and global numerical weather prediction models still must parameterize
the effects of subrgid-scale orography, which they cannot explicitly resolve. One of the effects are
the orography gravity waves that affect the dynamics and transport throughout the atmosphere due
to flux convergences during their dissipation. Complicating the problem further is the interplay with
the turbulence parameterization schemes, which influence the dynamics and mixing near the
surface and then aloft in unstable regions in the free atmosphere.
In this work, we study the life cycle of orography gravity waves numerically under background
conditions and set-ups ranging from idealistic to realistic. A hierarchy of idealized three-
dimensional simulations of mountain–flow interaction is developed for various orographic shapes,
atmospheric conditions and model settings (with turbulence parameterizations or in large-eddy
resolving mode) to address the coupling between orographic gravity waves and turbulence. The
ultimate goal of the study is to provide constraints for parameterized mixing in climate models and
establish foundations for coupling the turbulence and gravity wave parameterizations.

How to cite: Bartoň, Š. and Šácha, P.: Systematic analysis of flow-orography interactionin idealized numerical simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3384, https://doi.org/10.5194/egusphere-egu26-3384, 2026.

EGU26-4515 | ECS | Orals | AS1.23

Future alpine precipitation extremes under high-impact atmospheric circulation patterns 

Marc Lemus-Canovas, Alice Crespi, and Manuela Brunner

Understanding the behaviour of future extreme precipitation in the European Alps is a major adaptation challenge, as these events often cause flooding and severe impacts on infrastructure and society. Convection-permitting models (CPMs) have recently emerged as a key tool to better represent extreme precipitation processes in complex Alpine terrain, overcoming limitations of regional climate models (RCMs). While previous studies have analysed future changes in hourly and daily precipitation extremes using CPMs, it remains unclear how extremes will evolve under known impactful atmospheric circulation patterns, such as deep Mediterranean cyclones or persistent southerly flow regimes associated with major Alpine flood events.

Here, we investigate future precipitation changes conditioned on circulation types associated with observed high-impact events. We build on 6 impactful historical circulation types derived from the circulation classification scheme proposed in Lemus-Canovas et al. (2025). To identify circulation and   precipitation patterns analogous to these target circulation types, we apply a combined circulation–precipitation analogue framework. Candidate days are required to belong to the 10% closest circulation analogues, defined by the joint similarity of daily sea-level pressure and 500 hPa geopotential height fields simulated by each of the five EURO-CORDEX RCMs relative to the corresponding ERA5 circulation-type composite, quantified using a root-mean-square distance over the European domain. In addition, these candidate days must exhibit high precipitation-pattern agreement, defined as correlations exceeding the 90th percentile between CPM-simulated daily precipitation and an Alpine-wide observational precipitation dataset. Note that CPM outputs are first aggregated from hourly to daily resolution for the purpose of analogue selection. The final analogue dates are retained when basin-averaged precipitation exceeds the 90th percentile—computed separately for each experiment (Historical: 1996–2005; RCP8.5: 2090–2099) and weather type—if either 1-hour or 24-hour accumulated precipitation exceed the threshold in the most affected Alpine basins.

Our results show a precipitation intensification of autumn Mediterranean-origin weather types across all accumulation steps by the end of the century. For these circulation types, hourly precipitation extremes in CPMs scale with temperature   at or above the Clausius–Clapeyron rate (~7%/K), while weaker scaling is found at daily timescales. In contrast, summer-dominated weather types exhibit slight intensity increases at hourly scales but decreases at daily accumulations. These findings highlight strong circulation-dependent and scale-dependent changes in Alpine precipitation extremes and are particularly relevant for future risk management in the Alps.

References:

Marc Lemus-Canovas, Manuela Irene Brunner, Massimiliano Pittore, et al. Spatio-temporal patterns and drivers of high-impact precipitation events in the European Alps (1961-2022). ESS Open Archive . September 12, 2025. https://doi.org/10.22541/essoar.175767109.93227583/v1

How to cite: Lemus-Canovas, M., Crespi, A., and Brunner, M.: Future alpine precipitation extremes under high-impact atmospheric circulation patterns, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4515, https://doi.org/10.5194/egusphere-egu26-4515, 2026.

EGU26-4643 | ECS | Posters on site | AS1.23

Convection-Permitting Projections of Summer Extreme Precipitation Over the Tibetan Plateau 

Yongjun Chen, Wenxia Zhang, Liwei Zou, and Tianjun Zhou

Extreme precipitation is crucial for hydrological cycle and water resources, and has increased over many regions in recent decades. However, simulating and projecting precipitation extremes remain challenging over complex terrains, such as the Tibetan Plateau (TP). In this study, we evaluate the performance of the kilometer-scale (3.3 km) convection-permitting ICON model in simulating summer daily precipitation characteristics and extremes over the TP and project its future changes, focusing on the comparison with coarser-resolution CMIP6 models. ICON reasonably reproduces the observed daily precipitation characteristics, reducing the bias by ~80–95% for dry day frequency and precipitation-event persistence compared to ERA5 and the CMIP6 ensemble, and substantially lowering biases in extreme precipitation. For future projections, both ICON and CMIP6 project qualitatively consistent signals, including increasing extreme precipitation over almost the entire TP and, over the southeastern TP, increasing dry-day frequency and more frequent but shorter precipitation events. Despite consistent signs, ICON suggests an overall drier future over the southeastern TP than CMIP6, characterized by larger increases in dry days, smaller increases in extreme precipitation and event frequency, and a larger reduction in event duration. The systematic drier future in ICON compared to CMIP6 are linked to projected weakened low-level southwesterlies south of the TP, which suppress moisture transport into the interior southeastern TP and thus, reduce both daily and extreme precipitation. As water from southeastern TP affects downstream populations closely, these results are expected to provide more reliable projections for future risk assessments.

How to cite: Chen, Y., Zhang, W., Zou, L., and Zhou, T.: Convection-Permitting Projections of Summer Extreme Precipitation Over the Tibetan Plateau, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4643, https://doi.org/10.5194/egusphere-egu26-4643, 2026.

EGU26-4921 | ECS | Posters on site | AS1.23

From Global to Regional: The Added Value of High-Resolution Dynamical Downscaling for Precipitation in Southwest Asia's Complex Terrain 

Markella Bouchorikou, Thi Quynh Trang Nguyen, and Christoph Raible

Southwest Asia (SWA) is a climatically sensitive region where water resources are determined by the complex interactions between the Indian Summer Monsoon and Mediterranean winter systems. Coarse-resolution Global Climate Models (GCMs) have difficulties in capturing the arid-to-semi-arid hydroclimate of the region, which is characterized by high variability and orographically intensified precipitation. This study evaluates the added value of dynamical downscaling in representing mean and extreme precipitation in SWA. We use the Weather Research and Forecasting (WRF) model at a resolution of 10 km, driven by boundary conditions from the Community Earth System Model (CESM v1.2.2). For evaluating the models, we compare the native CESM (~2° resolution), the downscaled WRF simulation, and the ERA5 reanalysis for the common period 1950-2002. Our analysis reveals two outcomes for regional downscaling. First, the downscaled WRF simulation significantly improves the representation of the annual cycle, closely agreeing with ERA5, while the original CESM overestimates precipitation during summer. This overestimation can also be seen in the extreme precipitation values of CESM, especially in the south part of our region. Second, in areas of complex orography, like the Zagros Mountains, WRF tends to exaggerate precipitation compared to ERA5. Spatial differences between WRF and ERA5 precipitation in these complex regions can be attributed to the higher resolution of WRF. The extreme precipitation pattern generally agrees between WRF and ERA5 even though we observe the aforementioned spatial differences. The findings point out that dynamical downscaling can accurate simulate  topographically forced precipitation,  reducing large-scale GCM biases. This offers an important baseline for improved representation of precipitation in complex mountainous regions with low observational data availability, such as SWA.

 

How to cite: Bouchorikou, M., Nguyen, T. Q. T., and Raible, C.: From Global to Regional: The Added Value of High-Resolution Dynamical Downscaling for Precipitation in Southwest Asia's Complex Terrain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4921, https://doi.org/10.5194/egusphere-egu26-4921, 2026.

Although the concept of enhanced mountain warming has been around for several decades, it was not until just over a decade ago that the concept of elevation-dependent warming, whereby warming rates may be stratified by elevation, was widely identified by the scientific community as an important phenomenon. Unlike Arctic amplification, which is broadly homogenous, elevation dependent warming (EDW) is more complex, and although systematic changes in warming rates over the elevation gradient are often present, the pattern of the elevation profile is often non-linear and it can change with season, time of day and location. This is probably because there are a wide variety of drivers which can be responsible for contrasting warming rates, including patterns of surface albedo change (often driven by retreating snow cover and/or vegetation changes), aerosol loadings (and deposition on snow), changes in the free atmospheric lapse rate, Planck feedback and moisture controls on downward longwave emission (DLR) and clouds. In any one season or location, one or more of these drivers may have a dominant impact, leading to contrasting elevation patterns of change. 
Over recent years there has been an acknowledgement that elevation dependent changes involve broad adjustments in the climate system, which includes vertical gradients of precipitation, condensation, wind speed and shear, humidity and clouds. There has been a change in emphasis from EDW towards EDCC (elevation-dependent climate change). However our understanding of elevation dependent changes in variables other than temperature is in its infancy, in part because of lack of reliable observations at high elevations. Mountain precipitation (rain and snow) is particularly hard to measure accurately, and gridded datasets often interpolate to higher elevations based on limited observations. 
Future developments in EDCC research must involve both improving high elevation observations and learning from the new tranche of convection permitting models which can explicitly resolve more atmospheric processes such as mountain slope winds and small scale convection. Particular questions concern how orographic precipitation gradients may change, both for widespread stratiform precipitation and more intense localised convective storm development (often in summer). How the frequency and intensity of extreme events in mountain regions will change is also an important unanswered question, in particular how enhanced hourly precipitation extremes and heatwaves will be impacting high elevation regions. How EDCC will interact with the rate of snow loss and cryospheric change is also a major area of future concern, including impacts on downstream water supply. Other areas of EDCC research which have so far received relatively little attention include teleconnections with large scale circulation features such as the jet stream and Asian Monsoons, and interactions with ecological zonation and habitat hypsometry. The impact on mountain micro-climates, including the frequency, intensity and location of cold air pools is also not well understood. Thus, there are still numerous unanswered questions about climate change in mountain regions and at high elevations. 

How to cite: Pepin, N.: A decade of research in elevation dependent climate change (EDCC): A review of past discoveries and perspectives on future developments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5737, https://doi.org/10.5194/egusphere-egu26-5737, 2026.

EGU26-6475 | ECS | Posters on site | AS1.23

ERA5L Temperature validation in the Extended European Alpine Region 

Marco Bongio, Matteo Sangiorgio, and Carlo De Michele

Reanalysis products, like ERA5-Land, offer user-friendly, high-resolution gridded climate data (9 km) by combining ground observations, remote sensing, and model estimates. However, they inevitably contain uncertainties due to data gaps and modelling. Validating these datasets with land-based measurements is essential, though these observations also suffer from errors and inconsistencies. For this reason, this study validates ERA5-Land Temperature over the Extended European Alpine Region using the EEAR-Clim dataset, which includes only observational data records that meet strict reliability and temporal-consistency criteria.

The validation process involves 159 land-based meteorological stations, along with their corresponding nearest grid points in the ERA5-Land dataset. These grid points meet two criteria: a maximum elevation difference of ±100 meters and a maximum horizontal distance of ±0.5°. The selection procedure is designed to avoid repetition. The 159 grid points are different from each other. The stations are located between 504 and 2,965 meters above sea level and cover the period 1980–2020. We compared the daily temperature probability distributions for each station, grouping the stations into five elevation bands as well as considering the entire dataset. Our analysis examined temperature bimodality, the autocorrelation function, the ‘near-0°C probability’, and the ongoing issue of elevation-dependent warming trend.

The analysis shows that ERA5-Land generally underestimates temperature, with a global mean bias of –0.94 °C, and overestimates the standard deviation by +0.24 °C. The mean absolute error ranges from +1.37 °C in the lowest elevation band to +2.19 °C in the highest. The EEAR-Clim dataset provides clear evidence that low-elevation stations exhibit a bimodal temperature probability distribution, while stations above 1,500 m show a transition toward a unimodal distribution. ERA5-Land does not reproduce this transition, as even the highest grid points retain two main modes. The autocorrelation function of the observations decreases with elevation, whereas ERA5-Land shows increasing errors in its estimates, particularly at high elevations. The ‘near-0 °C probability’ is overestimated at low elevations and underestimated at high elevations. Despite this, the two datasets show good agreement in their estimates of the mean annual temperature trend rate, irrespective of elevation. However, the EEAR-Clim dataset indicates that lower elevations have warmed faster than the highest ones. These results are influenced by high variability and the limited number of stations above 2,000 m, which may affect or obscure the true temperature behavior. This underscores the urgent need for additional instrumentation, particularly at high elevations.

How to cite: Bongio, M., Sangiorgio, M., and De Michele, C.: ERA5L Temperature validation in the Extended European Alpine Region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6475, https://doi.org/10.5194/egusphere-egu26-6475, 2026.

EGU26-6720 | Orals | AS1.23

The impact of forest cover on the modeled valley atmosphere 

Manuela Lehner and Gaspard Simonet

The spatial resolution and accuracy of land-cover datasets used in numerical models can have a significant impact on the modeled mountain boundary layer. The land-surface cover influences the surface-energy budget through, for example, the effect of albedo on net shortwave radiation and roughness length on the turbulent exchange between the surface and the atmosphere. Local heating and cooling of the near-surface valley atmosphere are thus equally affected by the land-surface cover, which in turn influences the development of thermally driven slope and valley winds. In addition, the roughness length impacts near-surface turbulent momentum transport and flow fields, which may be of particular importance for shallow slope winds.

We have performed a series of WRF simulations for the Inn Valley, Austria, using three different land-use datasets and three idealized land-cover distributions. The two standard WRF land-use datasets MODIS and USGS strongly overestimate the amount of forest cover in the valley compared to the newer and better resolved CORINE Land Cover (CLC18) dataset. To further analyze the impact of this overestimation in forest cover, semi-idealized simulations are performed with a prescribed amount of forest cover across the model domain. The presentation will show the impact of the land cover on the local surface-energy budget and near-surface atmosphere as well as on the bulk valley atmosphere. Differences in the local sensible heat flux averaged over the surface of the valley are linked to total heating of the valley and the resulting valley-wind circulation.

How to cite: Lehner, M. and Simonet, G.: The impact of forest cover on the modeled valley atmosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6720, https://doi.org/10.5194/egusphere-egu26-6720, 2026.

EGU26-6869 | ECS | Posters on site | AS1.23

Exploring the complex dynamic of summer extreme events in the European Alpine Region using the high-resolution CORDEX-FPS ensemble 

Anna Napoli, Nikolina Ban, Claudia Pasquero, and Dino Zardi

Extreme summer precipitation events pose significant challenges, particularly in regions with complex topography such as the European Alps. Furthermore, the pronounced vulnerability of this region to climate change underscores the need to better understand its precipitation dynamics and processes at different spatial and temporal scales.

To in-depth investigate the spatial and temporal characteristics of these events, this study employs high-resolution regional climate simulations from the Coordinated Regional Climate Downscaling Experiment Flagship Pilot Studies (CORDEX-FPS) on convection over the Alps and the Mediterranean region. Focusing specifically on elevation-dependent patterns and sub-daily variability, we analyze the spatial distribution of summer precipitation extremes and the underlying processes associated with these events.

The results identify key hotspots of precipitation intensity and frequency, providing valuable insights for risk assessment, management, and adaptation strategies in mountainous regions. They also demonstrate how topography and other static factors, together with dynamic processes, affect the distribution of extreme precipitation events.

How to cite: Napoli, A., Ban, N., Pasquero, C., and Zardi, D.: Exploring the complex dynamic of summer extreme events in the European Alpine Region using the high-resolution CORDEX-FPS ensemble, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6869, https://doi.org/10.5194/egusphere-egu26-6869, 2026.

EGU26-7635 | Orals | AS1.23

On the proper use of near-surface temperature observations in atmospheric models deployed over mountain regions 

Isabelle Gouttevin, Danaé Préaux, Ingrid Etchevers, and Yann Seity

Near surface air temperature is a key meteorological parameter with high implications for the understanding and modelling of snow and water resource in mountain regions. Yet, it is hard to estimate and forecast accurately in these environments due to observational scarcity and model limitations in complex terrain.

In the present study, we analyze whether structural inhomogeneities in observational networks for temperature in mountain regions contribute to errors in their representations in numerical weather prediction (NWP) systems. Taking the case of the Arome-France NWP system over the French Alps, we analyze in particular the effects of the disparity in height above ground of the temperature sensors, of the inhomogeneous geographical distribution of stations that are preferentially located in valleys, and of the frequent altitude mismatch between stations’ real location and model grid points. We evaluate the consequences of these inhomogeneities in terms of model evaluation and data assimilation.

We especially show that measurement height is of high impact for model evaluation, providing a strong incentive to revisit model scores in mountain regions. It also carries strong implications for the assimilation, leading in the case of Arome-France to a negative impact of the assimilation of high-altitude temperature data if their height above ground is not properly considered. Inhomogeneities in data density between mountains and valleys also play a role that can be modulated depending on the assimilation system. This work paves the way for a better use of high-altitude near-surface observations within models deployed over mountain regions.

How to cite: Gouttevin, I., Préaux, D., Etchevers, I., and Seity, Y.: On the proper use of near-surface temperature observations in atmospheric models deployed over mountain regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7635, https://doi.org/10.5194/egusphere-egu26-7635, 2026.

EGU26-8111 | ECS | Posters on site | AS1.23

Anabatic Flows over Idealized Mountain Ridges and the Relation between Slope Angle and Turbulence Anisotropy 

Andreas Rauchöcker, Ivana Stiperski, and Alexander Gohm

Anabatic winds are thermally-driven flows that develop over heated mountain slopes. These upslope winds develop when the air near the slope rises due to the along-slope component of the buoyancy force, driven by the horizontal temperature contrast between the heated slope-adjacent air and the cooler ambient air at the same elevation. Due to the temperature difference, a horizontal pressure gradient forces the air to rise along the slope. Anabatic flows have a distinct vertical structure, with a near-surface wind maximum and a jet-like profile.

According to Prandtl’s analytical model and data from numerical simulations, the strength and depth of the anabatic flow layer are sensitive to the slope angle. The slope angle has also been suspected as a potential driver of turbulence anisotropy based on measurement results. The impact of the slope angle on turbulence anisotropy, however, has not been investigated in numerical simulations so far. To address this gap, we used the Cloud Model 1 (CM1) to conduct high-resolution large-eddy simulations of anabatic flows above idealized ridges to evaluate the influence of ridge height, slope angle and slope curvature on turbulence anisotropy. In total, 10 simulations have been conducted so far, consisting of 7 simulations for sinusoidal ridges of different heights, widths and slope angles and three simulations for ridges with the same constant slope angle but different ridge heights. The simulations were initialized with a constant potential temperature gradient throughout the domain and a constant surface heat flux of 0.12 K m s-1 and ran with a grid spacing of 10 m horizontally and 5 m vertically.

First results suggest that steeper slopes lead to more anisotropic turbulence. Apart from the slope angle itself, terrain curvature has a pronounced effect on the degree of anisotropy, as turbulence is more isotropic above slopes with constant slope angles compared to concave slopes of sinusoidal ridges. This is expected since upslope flow along a concave slope implies concave streamlines, and concave streamlines enhance shear stress and the momentum flux according to to the streamline curvature analogy. To gain further insights into the processes causing anisotropic turbulence, we plan to also investigate potential correlations between the degree of anisotropy and individual terms in the turbulent kinetic energy budget.

How to cite: Rauchöcker, A., Stiperski, I., and Gohm, A.: Anabatic Flows over Idealized Mountain Ridges and the Relation between Slope Angle and Turbulence Anisotropy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8111, https://doi.org/10.5194/egusphere-egu26-8111, 2026.

Coastal Santa Barbara is among the most wildfire-prone communities in Southern California. Downslope, dry, and gusty windstorms frequently occur along the south-facing slopes of the east–west-oriented Santa Ynez Mountains (SYM), which separate the Pacific Ocean from the Santa Ynez Valley. These winds, known as Sundowner Winds, typically peak after sunset and often persist overnight. They represent the most critical fire-weather phenomenon in the region.

The Sundowner Winds Experiment (SWEX), conducted from 1 April to 15 May 2022, integrated airborne and ground-based observations to examine interactions between continental and marine atmospheric boundary layers (ABLs), assess mountain waves and hydraulic jumps and their influence on surface winds and dew point, and evaluate forecasting challenges in mesoscale models.

This study analyzes two Sundowner events—IOP-2 (April 5–6) and IOP-10 (May 12–13)—affecting the eastern SYM. IOP-2 occurred during a heat wave, with temperatures reaching the 95th percentile, whereas IOP-10 reflected typical spring conditions.

During IOP-2, observations revealed sharp elevated inversions near the SYM, with mountain waves propagating across these layers. The free atmosphere was extremely dry, and strong horizontal winds were confined near inversion height. On the lee side, a large-amplitude lee wave evolved into a hydraulic jump, followed by wave breaking and a downslope jet. Despite strong offshore forcing, a shallow sea breeze developed over the eastern foothills, while nighttime marine boundary layer (MBL) intrusion—capped by a strong inversion—played a key role in the Sundowner cycle. Descending wave structures and rotor circulations produced reversed flows and enhanced surface winds. A nocturnal mid-channel eddy over the Santa Barbara Channel further stratified the MBL and decoupled it from the downslope jet. WRF simulations at 1-km resolution underestimated ridgetop and lee slope winds and overestimated coastal winds, with biases linked to misrepresentation of ABL height, inversion strength, and delayed MBL advection.

IOP-10 was investigated using ground-based instruments and radiosondes. It featured the second-largest observed mean sea level pressure difference between Santa Barbara and Bakersfield during SWEX. However, winds exceeding 20 m/s occurred on eastern slopes hours before peak pressure differences. LiDAR detected vertical motions near 6 m/s, associated with lifting of the lee-slope jet and weakening of surface winds—evidence of mountain wave activity influencing wind intermittency. Similar to IOP-2, the nocturnal mid-channel eddy contributed to lifting the lee jet and terminating Sundowners near the surface.

These findings emphasize the need for accurate representation of inversion structure and height, as well as marine–continental ABL interactions, in mesoscale models. Realistic simulation of complex flow dynamics—such as mountain waves and hydraulic jumps—is essential to improve forecasts of downslope winds in coastal environments. The SWEX campaign provided unique measurements to evaluate these features.

How to cite: Carvalho, L. M. V.: Downslope Windstorms in Coastal Mountains: Observations and Modeling during the Sundowner Wind Experiment (SWEX), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8550, https://doi.org/10.5194/egusphere-egu26-8550, 2026.

EGU26-8916 | Posters on site | AS1.23

East Asian Spring Precipitation and its Dry Trend revealed by CMIP6 High-Resolution Coupled Models 

Peng Zi, Jiandong Li, Ruowen Yang, Yimin Liu, ZihanYang Yang, Taohui Li, Bian He, and Qing Bao

The persistent spring precipitation over East Asia, with a notable drying trend in recent decades, poses substantial impacts on the regional hydrological cycle and socio-economy. This study investigates the climatology and long-term trend of East Asian spring precipitation during 1980-2014 simulated from CMIP6 HighResMIP coupled models, focusing on the role of model horizontal resolution. Our results show that high-resolution models outperform their low-resolution counterparts in simulating the spatial pattern and intensity of East Asian spring mean precipitation, owing to improved representations of low-level winds and moisture transport. However, many high-resolution models in HighResMIP fail to reproduce the long-term variation of East Asian spring precipitation and associated remote influencing factors (e.g., tropical Pacific and North Atlantic sea surface temperature) while only two models (FGOALS-f3-H and EC-Earth3P-HR) show improved performance for this unique climate phenomenon. Particularly, the high-resolution FGOALS-f3-H model exhibits the best skill in simulating this regional climatic change, increasing a regional mean drying trend from -0.10 in its low-resolution version to -0.33 mm day-1 decade-1 (observed: -0.43). This remarkable improvement in FGOALS-f3-H stems from more realistic representations of both the weakening Western North Pacific Anticyclone and strengthening Mongolia High, which are key regional circulation drivers of the East Asian spring drying trend, as well as its improved simulation of the weakening vertical velocity over East Asia. By contrast, five out of all seven high-resolution models show degraded performance in reproducing this precipitation trend, even showing amplified simulation biases in precipitation trend and improper relationships with remote and regional influencing factors relative to their low-resolution counterparts. This study suggests that the simultaneous improvement of horizontal resolution and physical parameterizations governing precipitation-related interannual variability in climate models is critical for simulating East Asian climatic change.

Keywords: East Asia, spring precipitation, high-resolution models, CMIP6

How to cite: Zi, P., Li, J., Yang, R., Liu, Y., Yang, Z., Li, T., He, B., and Bao, Q.: East Asian Spring Precipitation and its Dry Trend revealed by CMIP6 High-Resolution Coupled Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8916, https://doi.org/10.5194/egusphere-egu26-8916, 2026.

EGU26-9157 | ECS | Orals | AS1.23

Impact of black carbon on slope and valley winds in idealised simulations  

Johannes Mikkola, Victoria A. Sinclair, Giancarlo Ciarelli, Alexander Gohm, and Federico Bianchi

Thermally-driven valley circulation governs heat, momentum, and pollutant transport in mountains and is affected by the valley topography, large-scale weather, surface properties, and thermal forcing. Aerosols alter the heat distribution in the atmosphere through absorption and scattering of the incoming solar radiation, influencing the boundary layer (BL) development. From studies considering urban BL over flat terrain, it is known that depending on the radiative properties and vertical distribution of the aerosol population, aerosols can either enhance or suppress the buoyancy and mixing in BL, and cause simultaneous cooling and warming at different altitudes within BL. The impact of aerosols on the thermally-driven valley circulation remains poorly understood, a shortcoming addressed by this study.

This study examines how the absorption of incoming solar radiation by black carbon (BC) affects the daytime valley and slope winds in high-resolution idealised simulations using the Weather Research and Forecasting model coupled with chemistry (WRF-Chem). The simulations have an idealised valley topography that has a sinusoidal shape in the cross-valley direction and is 100 km long, 20 km wide, and 2 km deep. The study consists of two simulations: one including realistic BC concentrations interacting with the meteorological fields through absorption of shortwave radiation, and a reference simulation without BC. Heat and momentum budgets for the valley volumes are computed to understand the mechanisms behind the differences in the winds between the two simulations.

BC absorption acts to warm the upper BL and cool the lower levels during daytime, enhancing stability and reducing surface heating. Consequently, up-slope winds are weaker and confined to a shallower layer in the BC simulation. In the afternoon the up-valley winds are stronger in the BC simulation, although BC weakens the daytime temperature difference between the valley atmosphere and the BL above the plain. Based on the classic valley wind theory, the stronger temperature difference, hence a stronger pressure-gradient force, should lead to stronger up-valley winds. The average up-valley wind speed in the afternoon is 2.6 m s-1 in the BC simulation and 2.3 m s-1 in the simulation without BC. However, in the evening when the up-valley winds peak in magnitude, the maximum wind speed is stronger in the simulation without BC with a 0.5 m s-1 margin.

Momentum budget analysis shows that in the simulation without BC the pressure-gradient force is indeed stronger than in the BC simulation, which is in line with the stronger temperature difference. The advection term shows that the vertical export of along-valley momentum out from the valley by the cross-valley circulation, which is seen in the simulation without the BC, is suppressed or even absent in the BC simulation. This occurs likely due to the weaker up-slope winds which allow the stronger up-valley winds to develop in the afternoon despite the weaker pressure-gradient forcing. These results show that realistic BC concentrations can affect the thermally-driven valley circulation and fluxes of heat and momentum, revealing a pathway through which absorbing aerosols can modify the daytime slope and valley wind characteristics.

How to cite: Mikkola, J., Sinclair, V. A., Ciarelli, G., Gohm, A., and Bianchi, F.: Impact of black carbon on slope and valley winds in idealised simulations , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9157, https://doi.org/10.5194/egusphere-egu26-9157, 2026.

EGU26-10030 | ECS | Orals | AS1.23

Assessment of temperature variability over the Central System of the Iberian Peninsula: Multi-resolution model evaluation 

Sara Madera Sánchez, Fidel González Rouco, Elena García Bustamante, Jorge Navarro Montesinos, Cristina Vegas Cañas, Esteban Rodríguez Guisado, Ernesto Rodríguez Camino, Juan Carlos Sánchez Perrino, Ignacio Prieto Rico, Emilio Greciano Zamorano, Rita M. Cardoso Tavares, and Luana Cardoso dos Santos

Mountain regions are particularly vulnerable to climate change, as warming reduces snow and ice reserves, thus amplifying positive temperature feedbacks. These processes also have consequences for the hydrological cycle  and, therefore, having wide-ranging impacts on society by altering ecosystem services and products. This highlights the importance of understanding how climate change affects mountain areas. However, the limited availability of long-term climate records at high elevations, due to adverse weather conditions, makes high-resolution regional climate models essential for studying complex terrain. 


The CIMAs (Climate Research Iniciative for Iberian Mountain Areas) project is focused on analyzing climate variability and the impact of climate change on the Central System of the Iberian Peninsula. The studied area is the largest mountain range of the peninsula, reaching 2.592 m at its highest point (Almanzor Peak) and includes surrounding areas with lowest altitudes. 

CIMAs data is gathered from several institutions in Portugal and Spain and distributes over the domain of interest. It was used to asses the accuracy of two regional climate models: the WRF and the HCLIM models at 4 and 1 km horizontal resolution. Both were configured as convection permitting to allow for explicitly simulating convection. In addition, both models were driven by the same boundary conditions provided by the ERA5 reanalysis, which was also used to evaluate the added value of increased resolution by each regional model. 

Results show how increasing resolution improves the simulation of temperature at high elevations and allow for better understanding of the climatology of temperature in this mountain range. The comparison of the WRF and HCLIM simulations with observations highlights differences, mostly in the reproduction of extremes.

How to cite: Madera Sánchez, S., González Rouco, F., García Bustamante, E., Navarro Montesinos, J., Vegas Cañas, C., Rodríguez Guisado, E., Rodríguez Camino, E., Sánchez Perrino, J. C., Prieto Rico, I., Greciano Zamorano, E., Cardoso Tavares, R. M., and Cardoso dos Santos, L.: Assessment of temperature variability over the Central System of the Iberian Peninsula: Multi-resolution model evaluation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10030, https://doi.org/10.5194/egusphere-egu26-10030, 2026.

EGU26-10153 | ECS | Posters on site | AS1.23

Missing drag due to orographic gravity waves in a global numerical weather prediction model 

Hette Houtman, Miguel Teixeira, Suzanne Gray, Peter Sheridan, Simon Vosper, and Annelize van Niekerk

Various studies have shown that low-level drag in the atmosphere is parametrised inconsistently across the world’s numerical weather prediction and climate models, ultimately due to a lack of constraints on the underlying physical processes and the overlap in scale between them. Trapped lee waves (TLWs) are not parametrised in most models but have been shown in theoretical and case studies to produce significant drag (necessarily at low levels) on the atmosphere under the right conditions. To investigate whether TLWs contribute to low-level drag consistently, the resolved momentum fluxes in the archived analyses of the TLW-resolving UKV model are calculated and compared to the resolved plus parametrised gravity wave fluxes in the coarse-resolution, global version of the Met Office Unified Model (MetUM), which does not resolve TLWs.

The comparison between the models reveals that gravity wave momentum fluxes in the UKV model are about double that of the global MetUM in the mid-troposphere and up to four times that in the boundary layer. Only a portion of this discrepancy in momentum fluxes can be explained by the presence of trapped lee wave modes, which are found using a numerical solver of the Taylor-Goldstein equation. The other part is likely to be caused by orographic gravity waves that are reflected due to the general decrease of the Scorer parameter with altitude (and are distinct from the resonant TLWs). This work therefore demonstrates that the inclusion of the drag produced by both reflected and trapped lee waves would alleviate the current issues with low-level drag parametrisation.

How to cite: Houtman, H., Teixeira, M., Gray, S., Sheridan, P., Vosper, S., and van Niekerk, A.: Missing drag due to orographic gravity waves in a global numerical weather prediction model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10153, https://doi.org/10.5194/egusphere-egu26-10153, 2026.

EGU26-10268 | ECS | Posters on site | AS1.23

Differences in the Dominant Modes of the Interannual Variability of Eastern Tibetan Plateau Precipitation between Early and Peak Summers 

Erfan Liu, Song Yang, Haolin Luo, Jiehong Xie, and Ziqian Wang

The spatiotemporal variation of summer precipitation on the Tibetan Plateau (TP) is complex. In this study, we propose that there exist visible differences in the dominant modes of the interannual variability of eastern TP (ETP) precipitation between early (June) and peak (July–August) summers during 1979–2022. A north-south dipole pattern of the precipitation interannual variability appears in early summer, but in peak summer, the dominant mode is changed to be a monopole pattern. This phenomenon is mainly due to the intraseasonal transition of the dominant atmospheric circulation patterns over the TP and surrounding areas. In early summer, the north-south dipole pattern of the interannual variability of ETP precipitation is associated with the upper-level anomalous anticyclonic circulation over the western TP, which is primarily forced by the convective heating of South Asian summer monsoon. Under the control of anomalous northerlies on the eastern side of the anticyclonic circulation, the precipitation on the northern ETP is suppressed by both negative moist enthalpy advection and negative moisture advection. While in peak summer, the monopole pattern of the interannual variability of ETP precipitation is mainly regulated by the large-scale meridional displacement of the subtropical westerly jet. When the westerly jet shifts southward, the strengthened westerlies control the entire plateau and create unified positive moist enthalpy advection over the ETP, finally resulting in anomalous upward motions and increased precipitation; and vice versa. This study provides an insight that further investigations on the ETP summer precipitation should consider the intraseasonal difference. 

How to cite: Liu, E., Yang, S., Luo, H., Xie, J., and Wang, Z.: Differences in the Dominant Modes of the Interannual Variability of Eastern Tibetan Plateau Precipitation between Early and Peak Summers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10268, https://doi.org/10.5194/egusphere-egu26-10268, 2026.

Arctic mountainous environments show pronounced spatial and temporal variability in near-surface air temperature (Tair), driven by complex terrain, frequent temperature inversions, seasonal snow cover, and strong seasonal contrasts in solar radiation. Local atmospheric and surface processes, such as cold-air pooling, can cause rapid temperature changes over short distances and timescales. These dynamics are important for understanding Arctic ecosystem change and climate sensitivity, but remain difficult to quantify using sparse in situ temperature observations alone. Satellite-derived land surface temperature (LST) provides spatially continuous information on surface thermal conditions and has increasingly been explored as a proxy for Tair. However, LST-Tair relationships in Arctic mountain environments are highly variable, complicating the application of satellite LST for characterising fine-scale Tair patterns.

 

This study uses a unique in situ Tair dataset from the Kevo valley in northern Finland (26.88–27.05°E, 69.72–69.78°N), which is characterised by strong topographic shading, seasonal snow cover and frequent temperature inversions, and is subjected to the polar night and continuous summer daylight. The dataset comprises 65 stations spanning elevations from 74 to 330 m and recording hourly Tair since 2007. These observations are used to evaluate satellite‑derived LST and to develop models for mapping local Tair using Landsat LST combined with terrain and surface variables, including elevation, slope orientation, snow cover and vegetation indices. We analyse higher spatial resolution LST from Landsat sensors together with coarser resolution LST from MODIS Terra/Aqua and Sentinel-3 SLSTR, examining how terrain, snow cover and surface properties influence LST-Tair relationships and the ability of different LST products to represent microclimate variability across the valley. A focused case study examines high-resolution thermal patterns during nighttime and polar-night conditions using Landsat 8/9 LST acquired from October 2024 to August 2025. Preliminary results indicate that strong apparent LST-Tair agreement is largely driven by the seasonal cycle, with correlations in MODIS LST decreasing from ~0.95 to ~0.74 after deseasonalisation. For Landsat, performance is highly sensitive to data quality, with good‑quality data aligning closely with Tair and poorer‑quality data producing large scatter and a cold bias.

How to cite: Mo, Y., Pepin, N., and Lovell, H.: Mapping Arctic mountain microclimates using satellite land surface temperature: insights from the Kevo valley, northern Finland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10471, https://doi.org/10.5194/egusphere-egu26-10471, 2026.

EGU26-11637 | ECS | Orals | AS1.23

Coupling between Free Tropospheric Warming and Elevated Surface Warming 

Pietro Martuzzi and Marco A. Giorgetta

Elevation-dependent warming (EDW) has been reported in observations and climate models, yet its magnitude and controlling mechanisms remain uncertain, particularly due to the complexity of mountain regions. However both theoretical studies and climate simulations indicate a reduction in lapse rates and enhanced tropospheric warming under climate change. In this study, we examine EDW, and its relationship to tropospheric warming, in atmosphere-only experiments. This is done through the comparison between a historical control simulation and a perturbed climate state driven by uniform 4K warming in the prescribed sea surface temperatures. These simulations were performed with the ICON model in its Sapphire configuration at ∼10 km horizontal grid spacing. This setup offers an improved representation of high-elevation terrain compared to common climate change simulations, key to adequate analysis of EDW, together with a strong free-tropospheric warming, important for understanding its role in shaping EDW. 
The simulation exhibits a robust, statistically significant increase in surface warming with elevation, ranging from ∼4.9 K below 500 m to almost 7 K above 5500 m, corresponding to a global EDW slope of 0.317 K km-1. Regional contrasts are most pronounced at low elevations, while at intermediate and high elevations the surface warming profiles converge toward the tropospheric warming profile. Seasonal variations suggest an influence from snow-related processes, yet the majority of the seasonal variability in surface warming can be explained by seasonal variations in tropospheric warming.
A direct comparison of binned surface and tropospheric temperature changes at corresponding heights reveals a tight coupling, with small deviations possibly resulting from radiative processes near the surface. These results indicate that, under strong free-tropospheric warming, EDW can be approximated to first order by the vertical structure of tropospheric warming, with surface energy-balance processes largely providing secondary modulation. The sensitivity of this coupling to different forcing magnitudes and climate states warrants further investigation.

How to cite: Martuzzi, P. and Giorgetta, M. A.: Coupling between Free Tropospheric Warming and Elevated Surface Warming, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11637, https://doi.org/10.5194/egusphere-egu26-11637, 2026.

EGU26-11787 | Orals | AS1.23

Radiative impacts of particulate matter in a Himalayan valley: A modelling case study of the Khumbu Valley, Nepal. 

Giancarlo Ciarelli, Ludovico Di Antonio, Johannes Mikkola, Victoria A. Sinclair, Arineh Cholakian, Bertand Bessagnet, Tursumbayeva Madina, Angela Marinoni, Paolo Tuccella, and Federico Bianchi

Air pollution in mountain ecosystems has recently received particular attention. The peculiar and complex topography of such regions, combined with region-specific heating practices, has been shown to significantly reduce air quality levels, particularly in locations and communities situated on mountain valley floors.

The Khumbu Valley, located in the Himalayan ridge, connects the Indo-Gangetic Plain to the Nepal Climate Observatory – Pyramid (NCO-P) observation site at the foothills of Mount Everest (5079 m a.s.l). It often experiences high levels of particulate matter, including carbonaceous aerosols species (e.g. black carbon), which are largely modulated by the typical mountain valley circulation. These aerosols can be transported into the Khumbu valley from the Indo-Gangetic plain through thermally driven up-valley flows. However, the extent to which such circulation is directly impacted by absorbing and scattering aerosol compounds is currently unknown.

In this study, we conducted a one-month regional chemical transport model (CTM) simulation using the WRF-CHIMERE model at 1 km horizontal grid spacing, centered over the Khumbu Valley. The resolution was chosen to best account for the valley wind circulation typical of the region, while maintaining a trade-off with computational demands. We evaluated the impact of aerosols on meteorology due to aerosol-radiation interactions (ARI) over the Khumbu Valley and quantified its overall absolute magnitude. The pre-monsoon month of April was chosen as the period when transport of particulate matter from the Indo-Gangetic Plain is at its peak. Our results indicated that the model was able to reproduce the influx of particulate matter from the Indo-Gangetic Plain, with the modelled midday average peak in line with measurements at the NCO-P site. Accounting for ARI in the meteorological host model indicated a statistically significant cooling of the valley induced by aerosols, with potential implications for valley wind circulation. Given the extent of the Himalayan range, the results presented here may have implications for future climate scenarios, as aerosol-radiation interactions are often not resolved in coarse Earth system model applications.

How to cite: Ciarelli, G., Di Antonio, L., Mikkola, J., Sinclair, V. A., Cholakian, A., Bessagnet, B., Madina, T., Marinoni, A., Tuccella, P., and Bianchi, F.: Radiative impacts of particulate matter in a Himalayan valley: A modelling case study of the Khumbu Valley, Nepal., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11787, https://doi.org/10.5194/egusphere-egu26-11787, 2026.

EGU26-12250 | Posters on site | AS1.23

Optimizing Meteorological Station Placement for High-Resolution Field Reconstruction in Mountainous Terrain 

Anna Poltronieri and Nikolas Olson Aksamit

Reconstructing high-resolution geophysical fields from sparse observations is a central challenge for environmental sensing and model evaluation in complex terrain. While high-resolution climate models provide detailed insights, they are computationally expensive and difficult to validate in remote mountainous regions. This work adapts a data-driven sparse sensor placement framework [1] to identify optimized meteorological station locations for an arbitrary number of sensors in complex terrain.

Applied to a mountainous region in northern Norway, our approach can help hydrologists, glaciologists, and climate scientists determine where to place sensors to obtain independent streams of data, supporting a comprehensive representation of variables such as wind speed, humidity, or snow depth. We generalize the original framework by introducing a spatial weighting formulation, allowing users to prioritize specific sub-regions or account for physical constraints such as inaccessible terrain. In addition, prevailing wind patterns are incorporated into the selection criteria, guiding sensor placement toward configurations that capture the most frequent and impactful flow regimes. An orthogonal component approach is further introduced to integrate existing stations, ensuring that newly deployed sensors capture complementary information rather than redundant data. Ongoing work explores the use of the same framework to reconstruct missing or partially degraded measurements when stations are temporarily unavailable, using information from the remaining network.

A key advantage of the framework is its transparency. In contrast to many data-driven or machine-learning-based downscaling approaches, the reconstruction relies on explicit linear algebra operations, providing a traceable link from point observations to a domain-wide target field. For operational safety applications such as monitoring airport winds or avalanche hazards, this offers a computationally efficient and flexible alternative when high-resolution simulations are unavailable.

[1] Xihaier Luo, Ahsan Kareem, and Shinjae Yoo. “Optimal sensor placement for reconstructing wind pressure field around buildings using compressed sensing”. In: Journal of Building Engineering 75 (2023), p. 106855. issn: 2352-7102.

How to cite: Poltronieri, A. and Olson Aksamit, N.: Optimizing Meteorological Station Placement for High-Resolution Field Reconstruction in Mountainous Terrain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12250, https://doi.org/10.5194/egusphere-egu26-12250, 2026.

EGU26-13277 | ECS | Posters on site | AS1.23

Representing local-scale temperature patterns in complex terrain: performance of high-resolution datasets 

Elena Maines, Alice Crespi, Piero Campalani, Massimiliano Pittore, and Marc Zebisch

Gridded near-surface air temperature datasets are essential for environmental and climate applications, providing spatially continuous information beyond point measurements. In mountain regions, however, accurately representing temperature is particularly challenging. Strong spatial variability, frequent departures from simple elevation-based gradients, and cold-air pooling driven by nocturnal cooling and drainage flows lead to complex temperature patterns that are generally underrepresented when interpolating temperature observations from sparse weather stations. These limitations can reduce the accuracy in capturing extreme conditions, such as hot spells in the valley bottoms and urban areas or cold spells and strong thermal inversions. High-resolution dynamical models offer a complementary, physically based perspective by explicitly resolving terrain and atmospheric processes, improving representation of temperature gradients, diurnal cycles, and local circulations. Yet, near-surface temperatures in complex terrain remain sensitive to model resolution and surface-atmosphere coupling. The distinct strengths and limitations of these approaches raise the question of how different methods perform in representing local temperature patterns in complex terrain. In this study, we compare a 1-km dataset of daily near-surface air temperature produced through an interpolation scheme with high-resolution fields from dynamical modelling to assess the abilities to represent temperature variability in a complex mountainous terrain like the one of the Adige River catchment in Eastern Italian Alps. The interpolation method estimates the vertical temperature structure through a daily fitted, non-linear temperature-elevation profile based on more than 600 station observations at multiple altitudes and accounts for topographic complexity (Frei, 2014). Model-based products include the km-scale reanalysis VHR-REA_IT (Raffa et al., 2022) obtained by a dynamical downscaling of ERA5 for Italy at approximately 2-km resolution and the Copernicus European Regional ReAnalysis (CERRA). The comparison is conducted over the period 1990-2020 and focuses on the representation of temperature extremes and their spatial variability, e.g., cold-air pooling and heatwaves, and on the description of daily vertical profiles. Interpolated fields capture local extremes and cold-air pools where observations are available but are limited in resolving broader spatial variability and vertical thermal structure. In contrast, high-resolution reanalyses provide a more physically consistent depiction of thermal gradients, although systematic differences in describing extremes emerge. Our results will illustrate how the complementarity of approaches can guide the appropriate use and integration of temperature products in mountainous regions to support temperature-related hazard monitoring and risk assessment. 

How to cite: Maines, E., Crespi, A., Campalani, P., Pittore, M., and Zebisch, M.: Representing local-scale temperature patterns in complex terrain: performance of high-resolution datasets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13277, https://doi.org/10.5194/egusphere-egu26-13277, 2026.

EGU26-13515 | ECS | Posters on site | AS1.23

Recent high-altitude observations (2013-2024) of extreme air temperatures and associated atmospheric circulation patterns in the tropical Andes 

Tania Ita Vargas, Jean Emmanuel Sicart, Isabella Zin, Thomas Condom, Wilson Suarez, Kelita Quispe, Clementine Junquas, and Jhan-Carlo Espinoza

High-altitude mountains play a key role in modulating regional weather and climate. The tropical Andes in South America are characterized by strong climatic diversity and complex orography. In this region, identifying atmospheric circulation patterns (CPs) that control the meteorological extremes across different altitudinal and latitudinal gradients remains challenging. Using unique, quality-controlled hourly air temperature observations from four automatic weather stations located above 4700 m a.s.l. in the Peruvian Andes, this study links local extreme air temperature events to large-scale CPs during 2013-2024. CPs were identified using a k-means clustering algorithm applied to the standardized anomalies of the daily 200-hPa wind field from the ERA5 reanalysis over South America (10° N-30° S, 90°-30° W) for the 1980-2024 climatological period. Nine CPs were identified and classified into dry (D1-D4), wet (W1-W3), and transitional (T1-T2) circulation types, consistent with the regional seasonal cycle. Results show that warm nights (daily minimum air temperature exceeding the 90th percentile) are closely related to the occurrence of the transitional (dry-to-wet season) CP T1. This pattern is linked to warmer-than-normal conditions relative to the daily climatology, with a high frequency of warm nights observed from April to November. The 200-hPa circulation associated with T1 exhibits an upper-level ridge extending down to 500-hPa, resembling the Bolivian High. This circulation enhances easterly flow, favoring the advection of warm and moist air into the Andes and increasing nighttime and early-morning cloud cover. These conditions inhibit nocturnal radiative cooling and maintain elevated minimum air temperatures during a climatologically cold period in the Andes. During the 2023-2024 El Niño event, warm nights increased markedly compared to the previous years, while cold events became less frequent. This behavior appears to be primarily linked to an increased frequency of the T1 pattern, reaching up to 35%, particularly during July-October 2023 and April-July 2024. These findings provide a framework for future analyses of changes in this circulation regime under future climate scenarios and its role in modulating warm temperature extremes over the tropical glaciers.

How to cite: Ita Vargas, T., Sicart, J. E., Zin, I., Condom, T., Suarez, W., Quispe, K., Junquas, C., and Espinoza, J.-C.: Recent high-altitude observations (2013-2024) of extreme air temperatures and associated atmospheric circulation patterns in the tropical Andes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13515, https://doi.org/10.5194/egusphere-egu26-13515, 2026.

EGU26-14380 | Orals | AS1.23

Is bias correction necessary for CPRCM-driven flood simulation in mountainous region? 

Lu Li, Kun Xie, Hua Chen, Stefan P. Sobolowski, Øyvind Paasche, and Chong-yu Xu

Convection-permitting regional climate models (CPRCMs) at kilometer scale can better represent intense precipitation, yet their added value for flood-risk applications is still limited and often inconsistent. A key reason is the presence of systematic biases in precipitation and temperature over complex terrain, which may strongly affect hydrological response. To address whether bias correction is necessary when using CPRCM forcing for flood modelling in complex terrain, we run WRF-Hydro with raw and bias-corrected 3-km HCLIM3 precipitation and temperature for two contrasting basins spanning coastal to mountainous terrain in western Norway: Røykenes (coastal, rainfall-driven floods) and Bulken (mountainous, snowmelt-influenced floods). We further compare two widely used bias-correction approaches, i.e., Quantile Mapping (QM) and Distribution Delta Mapping (DDM), applied to precipitation and temperature prior to the hydrological simulations.

The results show that bias correction reduces mean biases in both variables, but its effectiveness depends on basin type and metric. In Røykenes basin, QM does not adequately correct annual maximum 1-hour precipitation, whereas DDM provides a better adjustment of extreme precipitation. For temperature, the correction reduces absolute bias relative to raw HCLIM3 but also shifts the bias from cold to warm. In terms of hydrological performance, raw HCLIM3 forcing already yields a small flood-peak bias in Røykenes basin (~3% underestimation), while bias-corrected forcing can further worse this peak underestimation. In Bulken basin, temperature correction improves both flood peaks and flood seasonality, underscoring the strong sensitivity of snowmelt-influenced floods to temperature errors. By contrast, precipitation correction in this mountainous basin degrades flood-simulation skill. Overall, our results show that CPRCM forcing can be highly informative for flood simulations, but the benefits depend on process regime: temperature correction is critical for snowmelt-dominated basins, while precipitation correction over mountains requires particular caution.

How to cite: Li, L., Xie, K., Chen, H., Sobolowski, S. P., Paasche, Ø., and Xu, C.: Is bias correction necessary for CPRCM-driven flood simulation in mountainous region?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14380, https://doi.org/10.5194/egusphere-egu26-14380, 2026.

EGU26-15032 | Posters on site | AS1.23

CIMAs: A multi-source climate dataset for high-mountain environments in the Iberian Central System 

Cristina Vegas Cañas, J. Fidel González Rouco, Esteban Rodríguez Guisado, Ernesto Rodríguez Camino, Rita M. Cardoso, Luana C. Santos, Jorge Navarro Montesino, Elena García Bustamante, Carlos Pereira, Yolanda Luna, Ana B. Morata, Guillermo Robles Martínez, and Jose A. Hinojal

The Climate research initiative for Iberian Mountain Areas (CIMAs) is a collaborative framework involving several Spanish institutions: the Spanish Meteorological Office (AEMET), Complutense University of Madrid (UCM), Institute of Geosciences (IGEO, CSIC-UCM) and CIEMAT. The main goal of the initiative is to advance the characterization and understanding of climate variability and change in the Central System of the Iberian Peninsula. Mountain regions are particularly sensitive to climate change, however observational data in these environments remain scarce, heterogeneous and difficult to maintain. CIMAs addresses this challenge by integrating multi-source meteorological datasets from institutions with different measurement protocols, temporal resolutions and data formats, such as AEMET, the Guadarrama Monitoring Network (GuMNet), the Portuguese Meteorological Office (IPMA), hydrological agencies operating Automatic Hydrological Information Systems in Spain (SAIH Duero, SAIH Tajo) and the Portuguese National Water Resources Information System (SNIRH). 

In this work, the development of the CIMAs observational database is presented. The workflow includes harmonization of formats and units, metadata consolidation, systematic quality control, temporal aggregation and a version-controlled architecture that ensures traceability and facilitates future updates. The temperature and precipitation databases are currently operational, incorporating station records distributed across Spain and Portugal. As part of the evaluation of the current data releases, spatial summaries of data availability and temporal coverage are also presented, together with preliminary climatological fields used to assess the internal consistency of the integrated datasets. The system additionally provides web-based tools for data visualization and access. Ongoing developments include the integration of wind and snow products and the coupling of the observational database with simulations. 

The CIMAs framework provides a structured and interoperable basis for integrating climate observations across high-mountain areas of the Iberian Peninsula. Its aim is to improve data accessibility, consistency and usefulness for scientific and operational purposes. In addition, it offers an observational basis for assessing simulation performance and for the development of climate-service applications.

How to cite: Vegas Cañas, C., González Rouco, J. F., Rodríguez Guisado, E., Rodríguez Camino, E., Cardoso, R. M., Santos, L. C., Navarro Montesino, J., García Bustamante, E., Pereira, C., Luna, Y., Morata, A. B., Robles Martínez, G., and Hinojal, J. A.: CIMAs: A multi-source climate dataset for high-mountain environments in the Iberian Central System, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15032, https://doi.org/10.5194/egusphere-egu26-15032, 2026.

EGU26-15938 | ECS | Orals | AS1.23

Ground validation of high-resolution WRF model precipitation estimates over Colombia 

Wesly Huertas, German Poveda, Kyoko Ikeda, and Roy Rasmussen

In this study, we perform a thorough validation of precipitation estimates from the high-resolution WRF model, run with a 4-km horizontal grid spacing over Colombia during 2000-2022, using in-situ data from the Colombia weather, climate and hydrology service (IDEAM) at annual, monthly, and diurnal scales. Model outputs were validated against IDEAM rain gauge data using multiple statistical metrics, including Spearman correlation, p-value, RMSE, ME, MAE, and BIAS.  Results show that the model is able to capture the main precipitation regimes, with notable contrasts between coastal (Caribbean and Pacific) and low-lying and plain regions (Orinoco and Amazon), and over the Andes cordillera. While the model generally tends to overestimate rainfall throughout most of the country, the error metrics are smaller over the Andean regions, where the spatial and seasonal variability are better represented. Comparisons across regions at monthly, interannual, and diurnal scales highlight significant differences between model estimates over the Pacific region and those over the Andes. The analysis includes the incidence of both phases of ENSO (El Niño and La Niña), showing positive and negative precipitation anomalies ranging between -300 mm and 350 mm per month, with higher anomalies during El Niño. Results of the validation at monthly and diurnal timescales highlight characteristic nighttime precipitation peaks consistent with the literature. These results confirm that, although the model effectively reproduces high-rainfall regions and their seasonal and diurnal variability, systematic biases remain, especially in the wettest periods (MAM and SON) underscoring the need for further calibration to improve its accuracy and practical applicability.

How to cite: Huertas, W., Poveda, G., Ikeda, K., and Rasmussen, R.: Ground validation of high-resolution WRF model precipitation estimates over Colombia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15938, https://doi.org/10.5194/egusphere-egu26-15938, 2026.

EGU26-16295 | Orals | AS1.23

A scale-adaptive parameterization of the horizontal wind field in the mountainous boundary layer 

Guang Li, Yuqi Feng, Hongxiang Yu, and Chenghai Wang

In mid-latitude regions, seasonal snow cover is predominantly distributed over high mountain areas characterized by complex terrain. Wind-driven snow transport is a key process controlling snow redistribution, accumulation patterns, and surface mass balance in these environments. However, a gap exists between the accurate representation of drifting snow processes, which requires boundary-layer wind fields at hundred-meter scales, and the coarse horizontal resolution of most atmospheric models on the order of 10 km, leading to large uncertainties in simulations of snow–atmosphere interactions in mountainous regions. In this study, multi-level nested simulations are performed using the WRF–LES framework to resolve boundary-layer horizontal wind fields across a range of spatial scales (from 9 km to 111 m) relevant to drifting snow. Wind speed statistics at different resolutions are analyzed, and their relationships with an integrated topographic factor are systematically quantified. Based on these analyses, a topography- and scale-dependent statistical downscaling scheme is developed to bridge the gap between coarse-resolution atmospheric forcing and fine-scale wind fields governing snow erosion, transport, and deposition. The result is also evaluated using in situ observations from a snow monitoring station in the Qilian Mountains, demonstrating an improved representation of near-surface wind characteristics, which are critical for snow redistribution.

How to cite: Li, G., Feng, Y., Yu, H., and Wang, C.: A scale-adaptive parameterization of the horizontal wind field in the mountainous boundary layer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16295, https://doi.org/10.5194/egusphere-egu26-16295, 2026.

EGU26-16406 | Posters on site | AS1.23

SPARTACUS version 3: An improved gridded climate dataset for Austria at daily resolution 

Yuri Brugnara, Angelika Höfler, Anna Rohrböck, and Ulrike Romatschke

SPARTACUS (Spatial Climate Observation Dataset for Austria) version 3 is the latest iteration of the main gridded dataset used by Geosphere Austria for operational climate monitoring. It provides daily values of temperature (mean, minimum, and maximum), precipitation sum, and sunshine duration at 1 km resolution for the territory of Austria and for selected surrounding regions (catchment areas of relevant rivers), covering the period from 1961 to the present. SPARTACUS is based solely on in-situ measurements of the Austrian network and of neighboring countries, which are interpolated by adapting statistical methods specifically developed for mountainous regions (e.g., Frei, 2014).

The most important addition with respect to the previous version (v2.1) is the calculation of the actual daily mean temperature (based on 24 hourly measurements) that replaces the arithmetic averages of maximum and minimum temperature. For the years preceding the automation of the measurements (when only three measurements per day are available) station-specific corrections were calculated by means of multi-linear regression to take into account a network-wide change of the observation times that took place in 1971 (Hiebl et al., 2025). In general, the temporal homogeneity of the input data has improved. Moreover, the number of ingested stations has been increased.

We demonstrate the improved suitability of the new version for climate‑change analyses compared to its predecessor (with particular focus on elevation-dependent climate change), examine the remaining issues, and offer an outlook on forthcoming developments.

 

References:

Frei, C. (2014), Interpolation of temperature in a mountainous region using nonlinear profiles and non-Euclidean distances. Int. J. Climatol., 34: 1585-1605. https://doi.org/10.1002/joc.3786

Hiebl, J., Rohrböck, A., and Haslinger, K. (2025), Correcting breaks in temperature and humidity observations: Implications for climate variability analysis in Austria. Int. J. Climatol., e70214. https://doi.org/10.1002/joc.70214

How to cite: Brugnara, Y., Höfler, A., Rohrböck, A., and Romatschke, U.: SPARTACUS version 3: An improved gridded climate dataset for Austria at daily resolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16406, https://doi.org/10.5194/egusphere-egu26-16406, 2026.

EGU26-16598 | ECS | Orals | AS1.23

 Modelling the black carbon dynamics over Almaty, Kazakhstan, during winter and summer seasons. 

Madina Tursumbayeva, Giancarlo Ciarelli, Ludovico Di Antonio, Manuel Bettineschi, and Nassiba Baimatova

Due to the close proximity of large urban areas to mountainous environments, air pollution can pose a serious threat to sensitive ecosystems through rapid transport driven by advection and mountain–valley circulation. Almaty (Kazakhstan), frequently ranked among the most polluted cities globally, is situated at the foothills of the Ile Alatau (part of the northern Tien Shan mountains). The city’s urban area located about 15-35 km from the major glacial systems, that have experienced a substantial decrease over the past years.  In this study, we investigated the impact of locally emitted black carbon (BC) from Almaty on the surrounding mountain areas using the WRF-CHIMERE regional chemistry-transport model with three nested domains up to 1 km resolution for periods representative of winter and summer conditions (i.e. January and July of 2023, respectively).

Simulation results indicated that during winter, BC concentrations remained trapped over the Almaty basin, at the lower elevations north of the city, and along the main valleys, due to stable atmospheric conditions and limited vertical mixing. In contrast, in summer, despite lower anthropogenic emissions arising from the city, BC was found to reach the mountain tops more effectively (up to 4000 m a.s.l.), likely due to increased vertical mixing and enhanced mountain–valley circulation. The peak BC concentrations at the mountain stations occurred approximately 5 (in July) – 8 (in January) hours after the maximum values in the city, suggesting faster upslope transport from the city in summer than in winter.

Additionally, model runs with and without online exchange between meteorology and chemistry were conducted to quantify the effect of BC concentrations on the radiative fluxes. Estimates of BC direct radiative effect (DRE) confirmed that the presence of BC over Almaty decreases solar radiation at the bottom of the atmosphere (BOA, BC DREBOA up to -1.20 W m-2) and enhances absorption within the atmosphere (BC DREATM up to +1.33 W m-2). Analysis of the potential temperature gradients in both months indicated, on average, no significant effect of BC concentrations on vertical atmospheric mixing, which in January can be attributed to strong temperature inversions over the region.

This research represents the first assessment of dynamics, transport and radiative effects of BC over the mountainous regions in Central Asia and highlights the need for further analysis extending to transitional periods (spring, autumn) when the temperature inversions are weaker or absent, but emissions rates remain high.

How to cite: Tursumbayeva, M., Ciarelli, G., Di Antonio, L., Bettineschi, M., and Baimatova, N.:  Modelling the black carbon dynamics over Almaty, Kazakhstan, during winter and summer seasons., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16598, https://doi.org/10.5194/egusphere-egu26-16598, 2026.

EGU26-20304 | ECS | Orals | AS1.23

Large scale atmospheric drivers of intraseasonal snowfall variability on Kilimanjaro's glaciers 

Robert Peal, Emily Collier, and Douglas Hardy

Due to the thermal homogeneity of the tropics, the rapidly retreating glaciers in Eastern Africa, such as at the summit of Kilimanjaro, are predominantly influenced by moisture and precipitation variability. Several case studies have shown that significant snowfall events with durations of just a few days can lead to deep snow cover that can persist for several months on the glaciers, with significant impacts on their long-term mass balance. However, the large-scale phenomena that influence this intraseasonal variability at high elevations remain poorly understood. Here, we use a unique dataset of daily surface height observations from Kilimanjaro’s Northern Ice Field and the ERA5 reanalysis to investigate the large-scale weather patterns that are associated with snowfall at the summit of Kilimanjaro from 2000-2022. We highlight that over 50% of surface height increase on the glacier was associated with the recently identified phenomenon known as westerly moisture transport events (WMTEs), atmospheric river like features that bring moisture into Eastern Africa from the Congo basin and can lead to enhanced precipitation in Eastern Africa. This work develops understanding of the processes that influence the mass balance of East Africa’s glaciers, which will help to improve the interpretation of these glaciers’ unique proxy record of the sparsely observed tropical mid-troposphere.

How to cite: Peal, R., Collier, E., and Hardy, D.: Large scale atmospheric drivers of intraseasonal snowfall variability on Kilimanjaro's glaciers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20304, https://doi.org/10.5194/egusphere-egu26-20304, 2026.

Complex terrain poses significant challenges for Numerical Weather Prediction (NWP) models, particularly in capturing localized boundary layer phenomena such as thermal circulations, katabatic flows, and temperature inversions. This study focuses on the Pyrenees mountain range, a region where accurate high-resolution forecasting is critical for understanding local weather extremes and variability, especially during synoptically quiescent conditions.

As part of a doctoral research project integrating Artificial Intelligence with high-resolution NWP, this work presents the foundational optimization of the Weather Research and Forecasting (WRF) model (v4.6.1). The modeling setup utilizes a one-way nested domain configuration bridging synoptic scales down to turbulence-resolving resolutions (333 m and 111 m LES), driven by ERA5 and GFS boundary conditions. We hypothesize that standard static input data provided by default in the WRF Preprocessing System (WPS) are insufficient to resolve the intricate surface heterogeneity of the Pyrenees. To address this, we conduct sensitivity experiments comparing the default USGS/MODIS configurations against enhanced high-resolution static datasets: 1-arc-second (~30 m) SRTM topography and the 100 m Copernicus Global Land Cover (CGLS-LC100). We evaluate the model’s performance in reproducing key local effects, focusing on surface wind fields, valley-floor cold pools, and thermal gradients under stable stratification.

Preliminary results quantify the bias reduction achieved by updating surface boundary conditions, establishing a robust baseline configuration. These findings are a prerequisite for subsequent full Large Eddy Simulations (LES) and the development of AI-driven bias correction schemes aimed at reducing computational costs while preserving accuracy in complex terrain.

This research has been funded by projects ARTEMIS (PID2021-124253OB-I00) and LIFE22-IPC-ES-LIFE PYRENEES4CLIMA.

How to cite: Toledano Rubí, A.: High-resolution WRF modeling in the Pyrenees: Sensitivity to static data for complex terrain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21196, https://doi.org/10.5194/egusphere-egu26-21196, 2026.

EGU26-1447 | ECS | Posters on site | CR7.3

Spatio-temporal patterns of dust storms and population exposure across land use and land cover types 

Yeganeh Soleimani, Hassan Dashtian, Amir AghaKouchak, Kaveh Madani, and Nima Shokri

Dust storms are driven by land-atmosphere interaction that transport dust and sand particles over vast distances. Dust storms have far-reaching impacts on air quality, ecosystems and human health, that affect hundreds of millions of people worldwide each year. Recognizing the importance of mitigating dust storm events and impacts, the United Nations has declared 2025-2034 as the Decade on Combating Sand and Dust Storms. However, a comprehensive understanding of the global distribution, seasonality, and land-surface controls of dust storm events remains limited, largely due to the lack of consistent ground-based, long-term, globally measured datasets.

NASA’s Atmospheric Infrared Sounder (AIRS) satellite provides a valuable global record of dust indicators, and analyzing these data enables large-scale tracking of where dust storm events occur and how their intensity evolves over time. In this study we analyze monthly dust storm data of AIRS satellite from 2003 to 2023 to show the global spatiotemporal trends in dust storms. In addition to mapping the spatial and temporal distribution of these events, we estimate the population affected by dust storms each year and assessed the intensity and frequency of these events across different land cover types. The study enables a better understanding of the regions and populations most at risk and provides valuable insights for policymakers and planners to develop strategies for mitigating the impacts of dust storms on human health, agriculture, and infrastructure.

How to cite: Soleimani, Y., Dashtian, H., AghaKouchak, A., Madani, K., and Shokri, N.: Spatio-temporal patterns of dust storms and population exposure across land use and land cover types, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1447, https://doi.org/10.5194/egusphere-egu26-1447, 2026.

Snow cover can significantly influence climate via modulating surface energy balance, yet its cross-seasonal impacts on Arctic temperatures remain poorly understood. Here, based on diagnostic analysis and numerical experiments, we reveal a robust linkage between reduced early spring (March-April) snow water equivalent (SWE) in northern Europe and increased May-June-July (MJJ) 2m air temperature over the East Siberian-Chukchi Sea during 1951–2022. Specifically, March-April SWE negative anomaly can persist to June and result in drier surface conditions due to reduced snowmelt. It led to elevated turbulent heat fluxes and positive geopotential height anomalies over northern Europe via snow-albedo and snow-hydrological effects during April-May-June. Hence, the eastward-propagating wave train enhanced over northern Europe and reaches South Siberia, causing cyclonic activity and enhanced precipitation. The resultant soil moisture increases persist into MJJ, favoring less sensible heat fluxes, upward wave activity flux, and wave train poleward-propagation. Finally, an anticyclonic anomaly appears over East Siberian-Chukchi Sea, enhancing anomalous descending motion, water vapor and downward longwave radiation, collectively raising near-surface temperatures. Moreover, numerical experiments successfully reproduce this cascade of mechanisms, confirming the physical pathway. Our study provides a new perspective for the studies of the snow cover climate effect, especially its impacts to the Arctic temperature variability.

How to cite: Wei, Z. and Ma, L.: Mechanism of Cross-Seasonal Response of Arctic Temperature to Eurasian Early Spring Snow Loss: The Critical Roles of Soil Moisture and Stationary Wave Propagation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2661, https://doi.org/10.5194/egusphere-egu26-2661, 2026.

EGU26-3486 | Orals | CR7.3

Drivers of observed winter–spring sea-ice and snow thickness at a coastal site in East Antarctica 

Ricardo Fonseca, Diana Francis, Narendra Nelli, Petra Heil, Joanathan Wille, Irina Gorodetskaya, and Robert Massom

Antarctic sea ice and its snow cover play a pivotal role in regulating the global climate system through feedback on both the atmospheric and the oceanic circulations. Understanding the intricate interplay between atmospheric dynamics, mixed-layer properties, and sea ice is essential for accurate future climate change estimates. This study investigates the mechanisms behind the observed sea-ice and snow characteristics at a coastal site in East Antarctica using in situ measurements in winter–spring 2022. The observed sea-ice thickness peaks at 1.16 m in mid–late October and drops to 0.06 m at the end of November, following the seasonal solar cycle. On the other hand, the snow thickness variability is impacted by atmospheric forcing, with significant contributions from precipitation, Foehn effects, blowing snow, and episodic warm and moist air intrusions, which can lead to changes of up to 0.08 m within a day for a field that is in the range of 0.02–0.18 m during July–November 2022. A high-resolution simulation with the Polar Weather Research and Forecasting model for the 14 July atmospheric river (AR), the only AR that occurred during the study period, reveals the presence of AR rapids and highlights the effects of katabatic winds from the Antarctic Plateau in slowing down the low-latitude air masses as they approach the Antarctic coastline. The resulting convergence of the two airflows, with meridional wind speeds in excess of 45 m s−1, leads to precipitation rates above 3 mm h−1 around coastal Antarctica. The unsteady wind field in response to the passage of a deep low-pressure system with a central pressure that dropped to 931 hPa triggers satellite-derived pack ice drift speeds in excess of 60 km d−1 and promotes the opening up of a polynya in the Southern Ocean around 64° S, 45° E from 14 to 22 July. Our findings contribute to a better understanding of the complex interactions within the Antarctic climate system, providing valuable insights for climate modeling and future projections.

How to cite: Fonseca, R., Francis, D., Nelli, N., Heil, P., Wille, J., Gorodetskaya, I., and Massom, R.: Drivers of observed winter–spring sea-ice and snow thickness at a coastal site in East Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3486, https://doi.org/10.5194/egusphere-egu26-3486, 2026.

Large-scale atmospheric circulation exerts a dominant control on the surface mass balance (SMB) of the Greenland Ice Sheet, yet circulation classifications are often optimized for atmospheric variability rather than for surface impacts. Here, we present an impact-oriented classification approach that emphasizes those regions of large-scale atmospheric circulation that are most relevant for Greenland’s SMB. Daily summer (June-August) 500 hPa geopotential height fields over a North Atlantic-Arctic domain encompassing Greenland are classified using self-organizing maps (SOMs). Prior to classification, the geopotential height fields are weighted based on their correlation with Greenland-wide SMB derived from a regional climate model (Modèle Atmosphérique Régional), such that regions exhibiting a strong linkage to SMB variability influence the circulation classification more. The weighting is derived from correlation patterns between geopotential height anomalies and Greenland-wide SMB anomalies, with a scaling factor systematically varied and selected to maximize both the separation of SMB characteristics across circulation regimes and the distinctness of the associated geopotential height composites. The resulting classification yields a set of circulation types that closely relate to differences in Greenland-wide SMB. Compared to unweighted SOM classifications, the impact-weighted approach enhances the separation of SMB responses across circulation regimes. By further analyzing the evolution of circulation regimes and their impact on Greenland’s SMB over time, we aim to improve understanding of changes in large-scale drivers relevant for the Greenland Ice Sheet mass loss.

How to cite: Fipper, J., Sasgen, I., and Abermann, J.: Connecting large-scale atmospheric circulation with Greenland's surface mass balance variability by impact-weighted self-organizing maps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3859, https://doi.org/10.5194/egusphere-egu26-3859, 2026.

EGU26-5491 | ECS | Orals | CR7.3

Attributing atmospheric phenomena driving Greenland Ice Sheet melt and their future changes 

Andrea Vang, Marco Muccioli, André Düsterhus, Hjalte Jomo Danielsen Sørup, Priscilla Mooney, and Jens Hesselbjerg Christensen

Compound warm and wet atmospheric events play a key role in driving extreme melt of the Greenland Ice Sheet (GIS), yet the relative contribution of different atmospheric phenomena remains poorly quantified. While atmospheric rivers (ARs) are frequently associated with extreme melt episodes, a systematic attribution of GIS melt to distinct types of atmospheric circulation features is still lacking.

Here, we apply a modified version of the Multi Object Analysis of Atmospheric Phenomena (MOAAP) tracking algorithm, optimized for Arctic conditions, to identify and track ARs, cyclones, jets, and frontal systems over Greenland. We quantify precipitation from each phenomenon. Together with temperature anomalies and surface melt, we relate these to individual phenomena and their compound occurrences. Extreme melt events are identified based on runoff, and attribution is performed by relating runoff to the presence and overlap of tracked phenomena over the ice sheet.

The analysis is applied to ERA5 reanalysis data and to PolarRES regional climate model projections. PolarRES includes a historical period and two RCP4.5 simulations representing distinct storylines. The first is characterized by enhanced Arctic amplification, which refelcts stronger local feedbacks. The second by reduced sea ice cover, which can indicate patterns of change is driven more by sea-ice loss and associated surface processes than by relative amplification of near-surface atmospheric warming. Using these scenarios allows us to investigate how differences in large-scale thermodynamic conditions may influence the atmospheric drivers of GIS melt, while applying the same phenomenon-based attribution framework across present-day and future climates.

By combining Arctic-optimized tracking of atmospheric phenomena with a GIS melt attribution framework, we investigate how extreme GIS melt events relate to specific atmospheric configurations and how these relationships may change under enhanced Arctic amplification or reduced sea ice. This study aims to improve our understanding of compound warm–wet events, their links to different types of atmospheric phenomena, and their role in GIS melt, as well as how they will shape the future GIS melt in climate projections.

How to cite: Vang, A., Muccioli, M., Düsterhus, A., Jomo Danielsen Sørup, H., Mooney, P., and Hesselbjerg Christensen, J.: Attributing atmospheric phenomena driving Greenland Ice Sheet melt and their future changes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5491, https://doi.org/10.5194/egusphere-egu26-5491, 2026.

EGU26-8348 | ECS | Orals | CR7.3

Impact of multi-mode and multi-species aerosols on 1D snow simulation at observational sites distributed at different latitudes. 

Sujith Krishnakumar, Martin Ménégoz, Samuel Albani, Christophe Dumas, Catherine Ottlé, Marie Dumont, Charles Amory, Philippe Conesa, and Yves Balkanski

Snow plays a critical role in energy budget by reflecting a significant portion of incoming solar radiation, thereby influencing local and global climate dynamics. However, the state-of-the-art climate models still face challenges to simulating global snow amount partly due to inadequate representation of snow albedo. Current models predominately parameterize snow albedo as an age-dependent, exponentially decaying function, which oversimplify its complexity. Also, most of these models neglect the deposition of aerosols (such as dust, black and organic carbons) and their ability of absorbing visible part of solar radiation, leading to reduced albedo and accelerated snowmelt. This “snow darkening effect” process is essential for improving the transient simulation of snow for climate and enhancing our understanding of climate feedback mechanism. To incorporate this phenomenon in ORCHIDEE, the land surface component of IPSL’s Earth System Model, we have implemented a comprehensive tracer framework that simulate the deposition and vertical transport of four log-normal modes of dusts, hydrophobic and hydrophilic black and organic carbons within snowpack. In order to enhance the snow aging processes, a snow metamorphism approach has been used that explicitly simulates the physical evaluation of snow optical diameter and sphericity, rather than relying on a simple chronological aging parametrization. To replace the empirically decaying albedo parametrization with a physics-based impure snow albedo, we have employed unique combination of Warren-Wiscombe’s uni-directional snow radiative transfer scheme with online optical property calculations of snow using Khokhanovsky’s scheme and mie-theory based offline aerosol optical properties. This enhanced physical representation of snow albedo dynamics. For validation against observation, offline ORCHIDEE simulations are conducted using in-situ meteorological forcing and MERRA-2 reanalysis aerosol deposition data across observation sites localized in different climatic areas over the Earth. These sites are selected to represent different aerosols regimes, each characterized by distinct dominant aerosol species. In these simulations, as snowpack develops seasonally, it harnesses aerosols deposited on the surface which are subsequently buried by additional snowfall and redistributed during melt-refreeze cycles. Consequently, snow albedo fluctuates, starting at high values following fresh snowfall and decreasing gradually due to increase in snow optical diameter (metamorphism) and accumulation of impurities, influenced by snow liquid content, vertical temperature gradient, aerosol species and deposition rate. The buried aerosols act as a memory and re-emerge at the surface in high concentration during the melting season. This re-exposure further reduces snow albedo, thereby accelerating melt rates. This simulated behavior is validated against in-situ observation of surface aerosol concentration and snow albedo. Through sensitivity experiments isolating the effects of different modes of dusts and other species, we further identified non-linear dynamics that critically influence the timing of snow melt and the end of the snow season.

How to cite: Krishnakumar, S., Ménégoz, M., Albani, S., Dumas, C., Ottlé, C., Dumont, M., Amory, C., Conesa, P., and Balkanski, Y.: Impact of multi-mode and multi-species aerosols on 1D snow simulation at observational sites distributed at different latitudes., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8348, https://doi.org/10.5194/egusphere-egu26-8348, 2026.

EGU26-8363 | ECS | Orals | CR7.3

A Vorticity-Based Climatology of Mesocyclogenesis Hotspots in the Southern Ross Sea 

Samira Hassani, Marwan Katurji, Peyman Zawar-Reza, Alena Malyarenko, and Alexandra Gossart

Polar lows (PLs) are intense small-scale cyclones whose detection remains challenging, limiting our understanding of their climatology. This study addresses this gap by developing an objective tracking algorithm to create a 35-year (1990-2024) climatology of potential PLs for the Southern Ross Sea using high resolution ERA5 reanalysis.

The method employs a multi-scale filtering approach to identify the key dynamical drivers and characteristic signatures of mesocyclogenesis. Potential systems are first detected using a primary dynamical criterion, defined by a significant maximum in 850-hPa relative vorticity, typically associated with an upper-level trough. Candidates are then filtered using a deep static instability criterion representing the thermodynamic contribution. The final selection retains features that exhibit canonical mesoscale characteristics of mesocyclones, including a compact vortex size, a short lifetime, strong surface winds, and a distinct negative mean sea level pressure (MSLP) anomaly. The results reveal that the primary regions for potential PL formation are concentrated along the Transantarctic Mountain coastline, with key hotspots near Terra Nova Bay, the Byrd Glacier and Siple Coast. The seasonal cycle is dominated by peaks in the transitional months of March and October, which represent the highest frequency of polar low candidates annually. A secondary, less pronounced peak in activity is observed during the mid-winter months of June and July. On an interannual scale, the climatology reveals a significant negative trend in summer PLs from 2008 to 2018. This decreasing trend is strongly correlated with a concurrent decline in regional atmospheric static instability, suggesting that a stabilization of the lower troposphere is a key driver of potential decline in PL number occurrence in the Ross Sea region. A key limitation of this vorticity-based approach is the potential for false positives, particularly the detection of shear-induced vorticity features that lack a coherent surface circulation.  This work creates the comprehensive, long-term, and objective climatology of mesocyclogenesis for the Ross Sea Region. This foundational dataset enables a quantitative analysis of the key drivers of mesocyclogenesis in the region. It provides a crucial benchmark for systematically investigating the interaction between large-scale atmospheric patterns, katabatic wind surges, sea ice extent, and topography in forcing high-latitude PLs activity, and for assessing how these relationships may shift under future climate change.

 

How to cite: Hassani, S., Katurji, M., Zawar-Reza, P., Malyarenko, A., and Gossart, A.: A Vorticity-Based Climatology of Mesocyclogenesis Hotspots in the Southern Ross Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8363, https://doi.org/10.5194/egusphere-egu26-8363, 2026.

The relationship between El Niño-Southern Oscillation (ENSO) and Southern Annular Mode (SAM) during austral summer is examined. It is found that their relationship is nonstationary and depends on the phase of the Interdecadal Pacific Oscillation (IPO). A strong ENSO-SAM relationship is observed during the positive IPO phase, while this relationship is weak during the negative IPO phase. The effects of sea surface temperature anomalies (SSTA) in the equatorial central-eastern Pacific, atmospheric stationary wave train, and synoptic-scale high-frequency eddies are found to be responsible for this interdecadal change in ENSO-SAM relationship. During the positive IPO phase, warm SSTA in the equatorial eastern Pacific associated with El Niño events induce a poleward-propagating wave train and cause an anomalous anticyclone over Antarctica. The anomalous baroclinicity to the north of the anomalous anticyclone is conducive to the eastward extension of eddy activity within the entrance of the mid-latitude jet stream, resulting in the development and maintenance of the negative SAM phase. However, during the negative IPO phases, the tropical SSTA centers during ENSO events shift towards the equatorial central Pacific, forcing the Rossby wave train that generates an anomalous anticyclone over the Ross-Amundsen Sea, to the north of that caused by ENSO during the positive IPO phase. Consequently, the anomalous baroclinicity does not align with the mid-latitude jet stream core, and the eddy-mean flow interaction at the jet stream cannot be effectively triggered, inducing a meridionally arched pattern confined to the Pacific-South American sector. Additionally, when the IPO and ENSO are out of phase (in phase), the superposition effect tends to amplify (dampen) the ENSO-SAM connection.

How to cite: Cai, X., Zhang, R., and Tan, Y.: Modulation of Interdecadal Pacific Oscillation on the Relationship Between El Niño-Southern Oscillation and Southern Annular Mode during Austral Summer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9116, https://doi.org/10.5194/egusphere-egu26-9116, 2026.

EGU26-9380 | ECS | Orals | CR7.3

On the relevance of serial cyclone clustering for Arctic sea ice 

Lars Aue, Sofie Tiedeck, Peter Finocchio, Timo Vihma, Petteri Uotila, Gunnar Spreen, and Annette Rinke

Short-term changes in Arctic sea-ice area are largely driven by weather events such as synoptic-scale cyclones, which typically cause ice loss during warm and stormy conditions in the Arctic. Physical mechanisms of this ice loss include enhanced sea-ice divergence, poleward ice drift, and changes in the surface energy budget due to advection of warm-moist air masses. In extreme cases, enhanced basal melt of sea ice occurs due to upward mixing of relatively warm ocean water. Such anomalous conditions are prolonged when several cyclones follow rapidly on each other, a phenomenon referred to as serial cyclone clustering. Serial cyclone clustering has been identified as a high-impact phenomenon, substantially amplifying wind damage, precipitation, and sea level extremes across several regions of the Earth. However, this weather phenomenon and its impacts have not yet been examined in the polar regions.

Here, we analyze changes in Arctic sea-ice concentration (SIC) for periods of serial cyclone clustering utilizing satellite observations and reanalysis data from 1979-2024. While cyclones generally decrease SIC compared to non-cyclone conditions in cold and warm seasons, the impact of cyclone clusters is approximately twice as strong and persists 2.5 times longer than for solitary cyclones. The amount of SIC-loss due to cyclone clusters scales with the intensity and number of clustered storms, and greater SIC-loss occurs during 2000-2024 compared to 1979-1999.

These findings emphasize the need to better understand drivers of serial cyclone clustering in the Arctic and more generally highlight the relevance of accumulated impacts of clustered weather events for Arctic sea-ice variability. Applying similar frameworks to other types of weather events and other target quantities (e.g. snow accumulation on sea ice or wind-driven ocean currents) could help to further sharpen our understanding of the role of weather extremes in the coupled polar climate system.

How to cite: Aue, L., Tiedeck, S., Finocchio, P., Vihma, T., Uotila, P., Spreen, G., and Rinke, A.: On the relevance of serial cyclone clustering for Arctic sea ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9380, https://doi.org/10.5194/egusphere-egu26-9380, 2026.

EGU26-10119 | ECS | Posters on site | CR7.3

The Role of the Southern Annular Mode and the El Niño-Southern Oscillation on Extreme and Unprecedented Antarctic Heat 

Charlie Suitters, James Screen, Jennifer Catto, Julie Jones, and Sihan Li

It was recently demonstrated using an ensemble of seasonal hindcasts with the “UNprecedented Simulated Extremes using ENsembles” (UNSEEN) technique that most of the Antarctic continent could experience record-breaking heat in both January and August. Here this analysis is continued, through the investigation of the role of large-scale modes of variability with known teleconnections to Antarctica, namely the Southern Annular Mode (SAM) and the El Niño-Southern Oscillation (ENSO), towards bringing relative warmth to Antarctica and its ice shelves during these months. The relationship between 2-metre temperature (T2m) and the SAM in the UNSEEN ensemble is consistent with the observed correlations: predominantly negative in both January and August. This negative correlation is strongest in magnitude along the coast of East Antarctica, while in the extreme north of the Peninsula a weaker positive correlation emerges. January correlations between T2m and ENSO are mostly positive in both observations and the UNSEEN ensemble, but spatial disparity between the two arises in August and perhaps suggests that the phase of ENSO could have a more varied influence on heatwave occurrence on different parts of the continent.

The polarity of the SAM dominates the Antarctic-wide mid-level circulation, and the teleconnection of ENSO is superimposed on top of this through modulation of the Amundsen Sea Low. This behaviour is identified in both observations and the UNSEEN ensemble. Therefore, for much of the continent heatwave days are dominated by negative SAM (SAM-) and are often combined with El Niño (EN) conditions. For example, SAM- patterns are more than twice as common during Antarctic-wide heatwave days than during all other days, and the combination of SAM- and EN is the most prevalent pattern that leads to heatwave days in the UNSEEN ensemble. However, in some locations (notably on ice shelves along the Peninsula) the relative occurrence of SAM- is no different between all days and heatwave days, and heatwaves occur with approximately equal probability across all combinations of SAM and ENSO phases. Strikingly, unprecedented T2m in Antarctica does not result from unprecedented SAM or ENSO values, suggesting either a deficiency in the UNSEEN ensemble, or that other processes not considered in this work are responsible for the most exceptional heatwaves in Antarctica. Further investigation into the large-scale drivers of unprecedented heat days in Antarctica is therefore required.

How to cite: Suitters, C., Screen, J., Catto, J., Jones, J., and Li, S.: The Role of the Southern Annular Mode and the El Niño-Southern Oscillation on Extreme and Unprecedented Antarctic Heat, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10119, https://doi.org/10.5194/egusphere-egu26-10119, 2026.

EGU26-11340 | ECS | Posters on site | CR7.3 | Highlight

Impacts of atmospheric rivers on major West Antarctic sea ice retreat in May 2025  

Michelle Maclennan, Michael Haigh, Caroline Holmes, Andrew Orr, Siddharth Gumber, Haosu Tang, Grant LaChat, Rebecca Baiman, Meghan Sharp, Paul Holland, Sihan Li, and Julie Jones

Sea ice acts as a dynamic membrane around the Antarctic continent, modulating atmosphere-ocean interactions and dampening the waves, precipitation, and heatwaves associated with poleward-propagating storms. In May 2025, intense wind and waves from an atmospheric river family wrought destruction on the Amundsen-Bellingshausen sea ice margin, leading to major sea ice retreat at the time of year typically marked by sea ice growth, and closing coastal polynyas.

In this study, we examine the linkages between anomalous atmospheric forcing and storm structure in May 2025, associated with the atmospheric rivers, and the resultant ocean response and sea ice retreat in the Amundsen Sea. First, we use ERA5 atmospheric reanalysis and satellite observations to classify the large-scale atmospheric drivers of the initial mid-May event and subsequent month-long marine intrusion conditions, including successive Rossby waves breaking and the buildup of a blocking high over the Antarctic Peninsula. Then, using the 1.5km resolution version of the atmosphere-only UK Met Office Unified Model (with sophisticated microphysics CASIM), we dynamically downscale ERA5 to examine the detailed vertical and spatial characteristics of the storm at the sea ice margin, including winds, air temperature, clouds, and rainfall and snowfall on sea ice. Finally, we examine the downstream, lasting impacts of the storm on sea ice, polynyas, and ocean temperature in the Amundsen Sea using a regional configuration of the Massachusetts Institute of Technology general circulation model (MITgcm) and satellite observations of sea ice concentration and drift.

Ultimately, after a monotonic decrease in extent from mid-May until mid-June, sea ice extent in the Amundsen-Bellingshausen sector never recovered in 2025. Our results suggest that individual atmospheric events can produce compounding impacts on the ocean and sea ice of the Amundsen Sea Embayment.

How to cite: Maclennan, M., Haigh, M., Holmes, C., Orr, A., Gumber, S., Tang, H., LaChat, G., Baiman, R., Sharp, M., Holland, P., Li, S., and Jones, J.: Impacts of atmospheric rivers on major West Antarctic sea ice retreat in May 2025 , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11340, https://doi.org/10.5194/egusphere-egu26-11340, 2026.

EGU26-11393 | ECS | Posters on site | CR7.3

Spatio-temporal variability of dust on snow: interactions with topography and snowpack dynamics observed with UAVs 

Pablo Domínguez Aguilar, Jesús Revuelto, Eñaut Izagirre, Javier Bandrés, Francisco Rojas Heredia, Pablo Ezquerro, and Juan Ignacio López Moreno

Aeolian dust surface deposition on seasonal snowpacks strongly influences snow albedo and melt dynamics, yet the environmental drivers of dust accumulation and redistribution at metre-scale resolution remain incompletely understood. UAV-based multispectral imagery enables detailed mapping of snow surface darkening associated with Light Absorbing Particles (LAP) such as mineral dust, offering new opportunities to investigate spatial distribution patterns in complex alpine terrain. This study examines the potential of UAV multispectral acquisitions to determine dust-on-snow spatial distribution and the relative influence of topographic factors on its variability during the seasonal evolution of the snowpack.

Data were collected in 2025 over a ~0.5 km2 alpine study basin in the Spanish Pyrenees using a MicaSense Altum multispectral sensor mounted on a DJI Matrice 300 UAV. Five UAV acquisition campaigns were conducted between initial Saharan dust deposition and snowpack melt-out. Spectral indices sensitive to snow surface darkening by LAP were computed from the UAV imagery. Additionally, from 10 to 20 distributed in situ snow surface samples were manually collected concurrently with UAV acquisition flights to determine surface LAP concentration and close-range spectral response using a hand-held hyperspectral radiometer to calibrate UAV-derived surface LAP concentration.

A suite of potential predictors to represent potential controls on surface LAP redistribution and accumulation were selected: elevation, slope, northness, topographic position index (TPI), maximum upwind slope (Sx), diurnal anisotropic heat index (DAH), snowpack depth and snowpack depth difference. Random forest (RF) models were applied independently to each acquisition date in order to assess how the relative importance of these controls evolved through time considering the different states of the dust layer in the snowpack.

The RF models generally reproduced the spatial variability of the LAP indices well, according to internal out-of-bag evaluation and the RMSE errors remained around low for days with larger LAP concentration variability. Throughout the study period, the state of the snowpack notably influenced the relative importance of the predictors to the response variable. We were able to observe days in which fresh snow partially covered the dust layer, causing predictor variables related to snow accumulation and elevation to show the highest relative importance. Subsequently, after the full surfacing of the dust layer, the largest LAP concentrations were found in concave areas, notably increasing the relative importance of TPI.

The results demonstrate the value of combining multi-temporal UAV multispectral observations with interpretable machine-learning approaches to account for the temporal sequence of dust deposition, burial, re-exposure, and melt to advance understanding of aeolian dust processes in alpine snow-covered environments.

How to cite: Domínguez Aguilar, P., Revuelto, J., Izagirre, E., Bandrés, J., Rojas Heredia, F., Ezquerro, P., and López Moreno, J. I.: Spatio-temporal variability of dust on snow: interactions with topography and snowpack dynamics observed with UAVs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11393, https://doi.org/10.5194/egusphere-egu26-11393, 2026.

EGU26-12591 | ECS | Orals | CR7.3

Curved atmospheric rivers and their moisture remnants: a new detection tool for Antarctica 

Victoire Buffet, Benjamin Pohl, Vincent Favier, and Jonathan Wille

Atmospheric rivers (ARs) represent the main intrusions of moisture and heat into Antarctica, exerting a major influence on the continent’s surface mass balance. Yet, due to geometric and directional constraints, existing detection algorithms often fail to track their evolution inland after landfall or in regions where abrupt directional changes occur. We introduce DARK (Detecting ARs using their Kurvature), a new Antarctic AR detection framework designed to overcome these limitations. DARK applies a strict 98th-percentile threshold to total integrated vapor transport and computes AR length along the curved axis to evaluate the 2000-km AR criterion. This enables the continuous detection of ARs with complex geometries, including those that curve, overturn, or extend across the South Pole. An additional AR-children module identifies smaller but still intense moisture remnants that detach from parent ARs after landfall yet continue to transport vapor and heat inland. The resulting climatology shows that DARK ARs account for about 18 % of total Antarctic precipitation and are linked to roughly half of top 1 % daily precipitation anomalies, 60 % of top 1 % daily maximum temperature anomalies, and 80 % of compound warm-and-wet events. DARK provides a more detailed assessment of AR-related precipitation and temperature impacts in the South Pole region. Despite slightly higher occurrence, risk-ratio analysis shows that DARK ARs more effectively capture the most intense events than earlier Antarctic schemes. Including AR-children further strengthens these associations, especially over Victoria Land, where they contribute to about one-third of AR-related precipitation.

How to cite: Buffet, V., Pohl, B., Favier, V., and Wille, J.: Curved atmospheric rivers and their moisture remnants: a new detection tool for Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12591, https://doi.org/10.5194/egusphere-egu26-12591, 2026.

EGU26-12689 | ECS | Orals | CR7.3

Quantifying the Radiative Impact of Light-Absorbing Particles on Alpine Snowpack Dynamics  

Sepehr Norouzi, Carlo De Michele, and Biagio Di Mauro

Light-absorbing particles (LAPs) such as black carbon, mineral dust, and organic carbon, when deposited on snow, reduce its surface albedo and increase the absorption of solar radiation. This enhanced absorption accelerates snowmelt and alters snowpack dynamics, particularly during the melt season. Field studies have measured seasonal concentrations of LAPs and confirmed their presence and significant effects on snow albedo. Even small quantities of LAPs can measurably reduce reflectance, particularly in the visible spectrum, and lead to earlier melt-out. A snowpack modeling assessment that isolates the individual and combined effects of each particle type under controlled scenarios can improve our understanding of their specific roles in snowpack evolution. Identifying the contribution of different LAPs to albedo reduction and snowpack dynamics is essential for alpine snow hydrology, where snowmelt timing governs runoff generation and water availability, and helps anticipate how LAPs-driven changes may amplify with climate change and reshape mountain hydrological regimes.

We first developed a one-layer energy budget snowpack model based on HyS (De Michele et al., 2013) and applied it over 18 hydrological years (2005–2023) at the Col de Porte experimental site in the French Alps, using local meteorological forcing. The model, referred to as HyS 3.0, was evaluated against long-term in situ measurements of snow depth and snow water equivalent (SWE), confirming its ability to accurately reproduce seasonal snow accumulation and melt dynamics. Due to its simplicity and low computational cost, HyS 3.0 is also well-suited for hydrological applications and sensitivity testing.

To assess the radiative effects of LAPs, we used field measurements of them along with spectral albedo data from two alpine sites Col de Porte (2014) and Col du Lautaret (2016–2018), capturing contrasting snow conditions. These datasets were used to evaluate BioSNICAR radiative transfer model performance, which computes snow albedo based on impurity concentration, grain size, and snow layer structure. After validation, BioSNICAR was used to generate a suite of LAP scenarios with varying concentrations and compositions. The resulting albedo changes were then used as input to HyS 3.0 to simulate the snowpack response under each scenario.

Results from these simulations revealed measurable changes in snowpack behavior, particularly in melt-out timing and snow specific surface area (SSA), compared to clean-snow conditions. This highlights both the direct radiative and indirect metamorphic effects of LAPs on seasonal snow evolution.

This work is supported by the “Light-Absorbing ParticleS in the Cryosphere and Impact on Water ResourcEs (LAPSE)” project, funded by MUR under the PRIN22 program.

How to cite: Norouzi, S., De Michele, C., and Di Mauro, B.: Quantifying the Radiative Impact of Light-Absorbing Particles on Alpine Snowpack Dynamics , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12689, https://doi.org/10.5194/egusphere-egu26-12689, 2026.

EGU26-12858 | ECS | Orals | CR7.3

Future Changes in Northern Hemisphere Extreme Snowfall 

Nick Romijn, Richard Bintanja, Eveline van der Linden, and Marlen Kolbe

While mean and extreme snowfall are projected to decline across many mid-latitude regions, particularly those close to the melting point. An opposing signal is expected in high-latitude and high-elevation regions, including the Arctic. Future changes in Northern Hemisphere extreme snowfall are investigated using KNMI’s Large ENsemble TIme Slice (LENTIS) model. Snowfall changes are closely linked to climate warming. Regional present-day seasonal mean climatological temperatures determine the sign of snowfall change through seasonally dependent temperature turning points. These turning points vary between -11℃ and -18℃ for median snowfall, whereas extreme snowfall exhibits higher turning-point temperatures ranging from -4 ℃ to -11℃ across seasons. As a result, increases in median snowfall event frequency and amount are confined to the coldest regions, while extreme snowfall is already increasing across a wider range of regions with higher climatological temperatures. Under warming conditions, sufficiently cold regions are projected to experience substantially larger increases in extreme snowfall frequency (up to 278%), and amount (up to 271%) than in median snowfall (up to 101%, and 152%, respectively). Regions that approach or exceed the melting point are primarily governed by thermodynamic effects, whereas colder regions remain influenced by a combination of thermodynamic and dynamical circulation changes. As snowfall is likely to influence the surface mass balance of the Greenland Ice Sheet, atmospheric circulation patterns over Greenland are examined in detail. Extreme snowfall over Greenland is found to occur predominantly during a dipole in sea level pressure anomalies spanning Greenland and Northern Europe, which promotes the northward transport of warm, moist North Atlantic air. Using the Greenland Oscillation Index (GOI), which quantifies the strength of this dipole, it is found that the projected increase in extreme snowfall is dynamically driven, with a higher frequency of circulation conditions, characterized by an above-median GOI, impacting particularly Eastern, Central and Northern Greenland. These future increases in extreme snowfall arise from more frequent favorable circulation patterns rather than from an intensification of circulation anomalies. 

How to cite: Romijn, N., Bintanja, R., van der Linden, E., and Kolbe, M.: Future Changes in Northern Hemisphere Extreme Snowfall, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12858, https://doi.org/10.5194/egusphere-egu26-12858, 2026.

EGU26-13334 | ECS | Orals | CR7.3

Impacts of High-Resolution Coupling of Solar Radiation Between Atmospheric and Cryospheric Components in Earth System Models 

Juan Tolento, Charles Zender, Andrew Roberts, Erin Thomas, and Mark Flanner

Earth system models (ESMs) often exchange solar fluxes and albedos between components using only two spectral bands (visible (VIS) and near-infrared (NIR)). In an effort to predict the albedo of cryospheric surfaces, which varies significantly through the NIR region, models often attempt to repartition these spectrally coarse incident solar fluxes into higher resolutions using prescribed, time-invariant weights. Here, we increase the resolution of solar fluxes and albedos exchanged between the atmosphere and snow-covered land surfaces within a fully coupled ESM from two bands to eight (one VIS and seven NIR bands). The exchange of higher resolution solar fluxes at the surface allows the surface models to dynamically weight the mean NIR albedo in response to time-varying atmospheric conditions. Diagnostic experiments within a fully coupled ESM show that the induced forcing on surface absorption caused by using the dynamic high resolution NIR insolation rather than prescribed weights ranges between -1.90-4.73 Wm-2. This forcing is strongly modulated by atmospheric humidity, as the presence of water vapor absorbs NIR radiation, thus changing the spectral distribution of NIR radiation at the surface, which cannot be captured with fixed weights. We find low/high humidity generally increases/reduces surface absorption. Regional climate responses over snow-covered surfaces are consistent with the applied forcing both in sign and magnitude. Replacing the coarse two-band surface albedo with an eight-band albedo better captures the steep drop of snow reflectance at longer NIR wavelengths, reducing the solar warming rate in the lower atmosphere. These advances provide a foundation for implementing a high resolution, spectrally consistent coupling of solar radiative fluxes across components within ESMs, demonstrating that increasing the spectral resolution of radiative processes yields a more physically realistic representation of albedo, surface absorption, and atmospheric absorption.

How to cite: Tolento, J., Zender, C., Roberts, A., Thomas, E., and Flanner, M.: Impacts of High-Resolution Coupling of Solar Radiation Between Atmospheric and Cryospheric Components in Earth System Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13334, https://doi.org/10.5194/egusphere-egu26-13334, 2026.

EGU26-13536 | ECS | Orals | CR7.3

A Comprehensive Snow Monitoring System to Detect the Impact of Rain-on-snow (ROS) at Ny-Ålesund, Svalbard  

Federico Scoto, Roberto Salzano, Mauro Mazzola, and Andrea Spolaor

In recent decades, the Svalbard archipelago has experienced the fastest warming on Earth, with rates approximately four times higher than the global average. Due to Arctic amplification, the weakening of the polar vortex, rising sea surface temperatures, and retreating sea ice have led to increasingly frequent intrusions of warm, moist air masses from the North Atlantic, resulting in winter temperature anomalies often accompanied by liquid precipitation. In turn, winter rain-on-snow (RoS) events have become more frequent and intense in recent years, causing complex and unprecedented interactions with ecosystems, hydrology, transportation, and infrastructure. Precipitation can substantially alter the physical state of snow cover by increasing liquid water content (LWC) and enhancing surface runoff, while refreezing of meltwater can form basal and internal ice layers, limiting accessibility to the underlying tundra for wildlife such as reindeer. In addition, RoS can also promote early seasonal snowmelt, altering nutrient release timing in Arctic ecosystems and increasing risk to local communities due to flooding and avalanches.

Although remote sensing and atmospheric reanalyses have proven effective for detecting RoS, accurate and reliable in situ measurements remain critical for bridging the multiscale gap . Ground-based snow data not only provide essential validation, but also offer the spatial and temporal resolution needed to resolve rapid, small-scale physical processes within the snowpack. To this end, a comprehensive snow observation system was installed in Ny-Ålesund (Western Spitsbergen, Svalbard) at the end of 2020, providing continuous, high-resolution measurements of several key parameters, including snow depth, SWE, albedo, and vertical profiles of snow temperature and LWC. Over the past five years, the system has been able to record both the seasonal evolution of the snowpack, generally lasting from November to the end of May, and the short-lived perturbations triggered by RoS events, improving our understanding of Arctic snowpack dynamics during extreme events. Here we present the instrumental setup, the main observational results collected between 2020 and 2025, and discuss the diagnostic parameters relevant for RoS process studies and model evaluation.

How to cite: Scoto, F., Salzano, R., Mazzola, M., and Spolaor, A.: A Comprehensive Snow Monitoring System to Detect the Impact of Rain-on-snow (ROS) at Ny-Ålesund, Svalbard , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13536, https://doi.org/10.5194/egusphere-egu26-13536, 2026.

EGU26-13762 | ECS | Orals | CR7.3

Evidence of Increasing trend of snow cover in himalayas implicate  snow darkening 

Saqib Ahmad Zargar, Chandan Sarangi, Priya Bhariti, Pranab Deb, Argha Banerjee, and Karl Rittger

While persistent snow cover traditionally preserves high surface albedo and buffers against early glacier melt, shifting precipitation regimes and light-absorbing aerosols are disrupting this protective mechanism. MODIS data indicates that the pre-monsoon snow season in the North Western Himalayas (NWH) extended by 7±3 days between 2000 and 2020. This extension is driven by large-scale dynamics, specifically moisture convergence and a deepened geopotential trough at 200 hPa.Crucially, snowfall resulting from these conditions enhances the wet deposition of atmospheric aerosols. As these aerosols resurface, they diminish the albedo benefits of fresh snow by 20%. This establishes a critical feedback loop wherein increased snowfall paradoxically facilitates surface darkening and accelerates melt. This snow-aerosol interaction necessitates a revision of surface energy balance models to accurately project future regional water availability.

How to cite: Zargar, S. A., Sarangi, C., Bhariti, P., Deb, P., Banerjee, A., and Rittger, K.: Evidence of Increasing trend of snow cover in himalayas implicate  snow darkening, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13762, https://doi.org/10.5194/egusphere-egu26-13762, 2026.

EGU26-14783 | Orals | CR7.3

Mineral Dust in Seasonal Snow and Firn on Svalbard Glaciers: Deposition Rates, Composition, and Albedo Impacts 

Susan Kaspari, Elisabeth Isaksson, Oscar Orme, Jean-Charles Gallet, Andy Hodson, William Hartz, Andrea Spoloar, Federico Scoto, Denise Diaz Vega, and Tess Kraics

Warming on Svalbard is occurring up to seven times faster than the global average and is driving widespread glacier retreat. In addition to rising air temperatures, light absorbing particles (LAP; including black carbon and mineral dust) can enhance snow and ice melt by reducing surface albedo. While black carbon has been studied extensively on Svalbard, mineral dust remains relatively understudied despite growing evidence that high latitude dust emissions may increase due to decreases in snow cover and glaciers retreat.

To address this knowledge gap, we analyzed mineral dust and black carbon in seasonal snow and firn cores collected from twelve spatially distributed Svalbard glaciers between 2022 and 2026. Dust concentrations and deposition rates were quantified using gravimetric filtration and ICP-MS, while dust mineral composition was characterized using X-ray diffraction and scanning electron microscopy with energy-dispersive spectroscopy. Black carbon was measured on select firn samples using a Single Particle Soot Photometer.

Results show pronounced seasonal variability, with low winter dust concentrations and enhanced summer–fall deposition, as well as substantial spatial variability in dust concentration, mineralogy, and spectral reflectance. Winter dust concentrations ranged from 0.3 to 17.6 µg g⁻¹ (median 0.9 µg g⁻¹), with deposition rates between 0.1 and 1.5 g m⁻² (median 0.4 g m⁻²). Mineralogical analyses reveal abundant sheet silicates and common rock-forming minerals across all sites, with carbonates largely restricted to central Svalbard glaciers, indicating variability in dust sources and depositional processes. Radiative transfer modeling demonstrates that mineral dust dominates LAP driven albedo reductions, exceeding contributions from black carbon. These findings highlight the growing importance of mineral dust for Svalbard snow and ice melt in the warming Arctic.

How to cite: Kaspari, S., Isaksson, E., Orme, O., Gallet, J.-C., Hodson, A., Hartz, W., Spoloar, A., Scoto, F., Diaz Vega, D., and Kraics, T.: Mineral Dust in Seasonal Snow and Firn on Svalbard Glaciers: Deposition Rates, Composition, and Albedo Impacts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14783, https://doi.org/10.5194/egusphere-egu26-14783, 2026.

EGU26-14921 | ECS | Posters on site | CR7.3

Extreme events and impacts of High Latitude Dust  

Pavla Dagsson Waldhauserova, Outi Meinander, and IceDust members

Sand and dust storms, including High Latitude Dust (HLD), were identified as a natural hazard that affects 11 of the 17 Sustainable Development Goals. HLD is a significant contributor to land degradation, severe erosion and ecosystem collapse, as documented for example in Iceland. HLD contributes to Arctic Amplification, and it was recognized as an important climate driver in Polar Regions (IPCC SROCC, 2019; AMAP, 2021). HLD has impacts on climate, such as effects on cryosphere, cloud properties, atmospheric chemistry and radiation, and marine and terrestrial environment. Main socio-economic sectors such as health protection, road safety, energy production, aviation, and land degradation, are negatively impacted by HLD (eg. severe air pollution, mortality on roads due to reduced visibility).

Many extreme events causing severe air pollution were observed and measured in Iceland, Svalbard and Antarctica. In Iceland, we measured i. tens of severe dust storms at multiple locations annually as well as long-range transport from Iceland to Scandinavia, Faroe and British Isle, and Svalbard; ii. Snow-dust storms; iii. Saharan dust plumes causing air pollution in Iceland; iv. Extreme wind erosion events of volcanic ash mixed with dust; v. dust storms during high precipitation/low wind periods; vi. Dust storms during glacial outburst floods, vii. Arctic winter dust storms during Polar Vortex conditions, and viii. Black/Organic Carbon haze from burning mosses around the eruption in Reykjanes Peninsula, transported > 300 km to Northeast Iceland. Several dust storms were measured also in Antarctic Peninsula. In Svalbard, aerosol measurements revealed high concentrations of both dust, coal dust and Black Carbon, while dirty snow evidenced the occurrences of Snow-Dust Storms, similarly to Iceland.    

In-situ particulate matter data and observations from these extreme events will be presented. It is crucial to provide long-term daily aerosol measurements and dust forecasts from the remote high latitude dust regions. Additional in-situ observations around HLD sources would confirm that the background air quality is not as good as expected, and in some cases, it is worse than industrial or some urban stations, such as in Iceland during the CAMS NCP Iceland projects.

More information and activities of HLD networks can be found at the Icelandic Aerosol and Dust Association (IceDust) websites (https://ice-dust.com/, https://icedustblog.wordpress.com/publications/), UArctic Network on High Latitude Dust (https://www.uarctic.org/activities/thematic-networks/high-latitude-dust/), NORDDUST (https://ice-dust.com/projects/norddust/), and CAMS NCP Iceland (https://ice-dust.com/projects/cams-ncp-iceland/, https://atmosphere.copernicus.eu/iceland).

How to cite: Dagsson Waldhauserova, P., Meinander, O., and members, I.: Extreme events and impacts of High Latitude Dust , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14921, https://doi.org/10.5194/egusphere-egu26-14921, 2026.

EGU26-16196 | ECS | Orals | CR7.3

Climatology of Atmospheric Rivers-related precipitation over different surface types in the Southern Ocean 

Melanie Lauer, Christopher Horvat, Michelle McCrystall, and Anna Possner Lowdon

Antarctica experienced a rapid decline in sea ice extent in 2016 following a modest increase in annual sea ice extent. Rapid changes in Antarctic sea ice have consequences for the Antarctic climate system; however, the coupled atmosphere-ocean-ice processes driving these changes remain poorly understood. Precipitation is a key atmospheric variable influencing both the surface mass balance of the Antarctic ice sheet and the formation and persistence of Antarctic sea ice.  Two major moisture sources contribute to precipitation: local evaporation due to the reduced insulation effect of sea ice and poleward moisture transport from lower latitudes, often associated with atmospheric rivers (ARs) – long, narrow corridors that transport large amounts of heat and moisture from the mid-latitudes to the polar regions. 

Despite their rarity, ARs play an important role in the Antarctic climate system, contributing to surface melt on the West Antarctic Ice Sheet and extreme precipitation events across East Antarctica. However, the role of ARs and AR-related precipitation, particularly in relation to Antarctic sea ice, has been less explored. 

Here, we analyze ERA5 reanalysis data to investigate the contribution of ARs to precipitation over the Southern Ocean (60 – 90S), distinguishing between different surface characteristics (open ocean and sea ice) and precipitation phase (rain and snow). Our results show that ARs contribute more to rainfall (50%) than snowfall (25%). AR-related snowfall is relatively evenly distributed across the entire study region, whereas around 75% of AR-related rainfall occurs over the Ross Sea and Amundsen-Bellingshausen Seas. While AR-related snowfall exhibits weak seasonal variability, AR-related rainfall is more pronounced in winter and spring. Regarding different surface types, AR-related rainfall primarily occurs over the open ocean throughout the year but extends over sea ice during winter. In contrast, AR-related snowfall shifts seasonally, dominating over the open ocean in summer and autumn and over sea ice in winter and spring.  

Area-normalized precipitation reveals that AR-related precipitation events are more intense than non-AR events, with higher intensities in winter compared to summer.  These findings highlight the important role of ARs and their potential changes in Antarctica. Finally, we compare these results with simulations from the newly developed climate model ICON-XPP to assess its ability to represent AR characteristics over the Southern Ocean.

How to cite: Lauer, M., Horvat, C., McCrystall, M., and Possner Lowdon, A.: Climatology of Atmospheric Rivers-related precipitation over different surface types in the Southern Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16196, https://doi.org/10.5194/egusphere-egu26-16196, 2026.

EGU26-17359 | ECS | Posters on site | CR7.3

Impact of Motion Correction on Momentum and Sensible Heat Fluxes over Ice and Water Measured on a Moving Vessel in the Arctic 

Florian Fröhlich, Theresa Mathes, Sabine Lüchtrath, Philipp Oehlke, Holger Siebert, Birgit Wehner, and Andreas Held

The Arctic exhibits an alarming warming rate, mainly caused by increasing greenhouse gas emissions and the climate forcing effect of aerosols. To get a better understanding of the relevance of local aerosol sources and sinks in the Arctic, vertical near-surface particle, momentum and sensible heat fluxes were investigated by collecting a large eddy covariance data set including three-dimensional wind speed, temperature and particle number concentration over ice, water and mixtures thereof during the PS131 expedition of the German research icebreaker Polarstern in 2022 using a 3-axis ultrasonic anemometer (Gill Solent HS-044, Lymington, United Kingdom) and a mixing condensation particle counter (Brechtel Model 1720, Hayward, USA). Both instruments were installed on the bow crane outrigger.

To minimize the influence of the inadvertent movement of the vessel caused by waves and wind on the anemometer data, two separate motion correction approaches were tested. The first method is based on the work of Fujitani (1981) and Edson et al. (1998). It realigns the wind vector (u, v, w) recorded in the vessel coordinate system with a reference frame while also correcting for apparent winds resulting from the tilting motion and the vessel movement in the reference coordinate system itself. Alternatively, by making use of the periodicity of the vessel movement and finding the frequencies with which the vertical wind vector component w oscillates using spectral FFT analysis, affected frequencies can be replaced assuming spectral similarity of atmospheric turbulence. Thus, it is possible to remove the impact of the movement without having to rely on the measured pitch, roll and yaw angles.

Both approaches were successfully used to correct the recorded data in preparation for calculating the sensible heat and momentum fluxes. Preliminary results suggest that the choice of motion correction approach has an impact on the obtained fluxes, though a complete evaluation of the resulting data is still pending at the time of abstract submission.

This study was funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation): HE5214/10-1, HE5214/11-1 and WE 2757/6-1.

How to cite: Fröhlich, F., Mathes, T., Lüchtrath, S., Oehlke, P., Siebert, H., Wehner, B., and Held, A.: Impact of Motion Correction on Momentum and Sensible Heat Fluxes over Ice and Water Measured on a Moving Vessel in the Arctic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17359, https://doi.org/10.5194/egusphere-egu26-17359, 2026.

EGU26-17631 | Orals | CR7.3

Drivers and Impacts of Extreme Weather Events in Antarctica: Recent Results and Future Plans of the ExtAnt Project 

Tom Bracegirdle, Sammie Buzzard, Will Dow, Danny Feltham, Neven Fučkar, Amelie Kirchgaessner, Hua Lu, Amanda Maycock, Andrew Orr, Sarah Shannon, Shivani Sharma, Martin Widmann, and Ryan Williams

In recent years a number of record-breaking, even record shattering, extreme weather and climate events have occurred over Antarctica. Such events can drive increased surface melt, thinning and even break-up of Antarctica’s ice shelves. They also pose threats to Antarctic species, ecosystems and the globally important services they provide. However, our knowledge and understanding of how extreme events over Antarctica may respond under climate forcing is lacking. To addresses this gap, the ExtAnt project is an ambitious four-year programme of research that brings together leading UK and international scientists to use new modelling resources and methods to elucidate drivers of extreme events in Antarctica. It aims to provide a comprehensive assessment of present day and future high impact extreme weather events in Antarctica, and associated risks. Key foci for impacts are surface melt on ice shelves and the highly specialised Antarctic biodiversity.

Recent science highlights will be presented on characteristics and drivers of extreme events and a new database of Antarctic extremes. An example of current early initial analysis relates to large ensembles, which shows that global climate models exhibit larger biases in mid-tropospheric daily meridional wind extremes at 65°S in summer (too weak) than in winter, in contrast to larger winter biases in the mean climatology. There is a fairly small, but clear, increase in the magnitude of meridional wind extremes in summer in the ozone hole period compared with the pre-ozone period. Wider implications the results so far will be discussed along with future plans for the project in downscaling (using both machine learning and traditional approaches), event attribution and surface melt modelling.

How to cite: Bracegirdle, T., Buzzard, S., Dow, W., Feltham, D., Fučkar, N., Kirchgaessner, A., Lu, H., Maycock, A., Orr, A., Shannon, S., Sharma, S., Widmann, M., and Williams, R.: Drivers and Impacts of Extreme Weather Events in Antarctica: Recent Results and Future Plans of the ExtAnt Project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17631, https://doi.org/10.5194/egusphere-egu26-17631, 2026.

EGU26-17638 | Orals | CR7.3

Experimental Reduction of Snow Surface Albedo by Local Black Carbon and Mineral Dust Deposition in the Andes of Laguna del Maule, Chile 

Tomás R. Bolaño-Ortiz, Felipe McCracken, María F. Ruggeri, Lina Castro, Luciano A. González-Faune, José A. Neira Román, Fredy A. Tovar-Bernal, and Magín Lapuerta

Snowmelt from the Andes is the primary source of freshwater for central Chile, a region experiencing prolonged drought and increasing anthropogenic pressures. Light-absorbing particles (LAPs), such as black carbon (BC) from mining vehicles and locally derived mineral dust (MD), accelerate snowmelt by reducing surface albedo. This study presents experimental results from a field campaign conducted on 27 August 2025 near Laguna del Maule, where controlled deposits of BC and MD were applied to the snow surface to quantify their impact on spectral albedo. BC (simulating mining truck emissions) and MD (local soil) were deposited cumulatively at masses of 1, 2, 3, 5, and 7 grams over a defined snow area. Surface albedo was measured using a spectroradiometric system consisting of six synchronized spectroradiometers covering 300–2500 nm. For each contamination level, 12 replicate measurements were taken. Broadband albedo (300–2500 nm) was averaged across replicates to evaluate the reduction induced by each LAP type. Due to wind-driven dispersion, the average effective mass deposited on the snow surface was 58% of the applied BC and 93% of the applied MD. Results show a consistent decrease in average broadband albedo with increasing deposition mass. A linear regression between broadband albedo and the effective surface concentration (accounting for wind loss) yielded an average albedo reduction slope of 0.014 ± 0.002 per gram of BC and 0.011 ± 0.001 per gram of MD. This indicates that, under these experimental conditions, BC exerts a stronger per-mass darkening effect than MD. These findings demonstrate that vehicular BC and wind-blown MD from mining and disturbed soils can significantly darken snow surfaces, thereby enhancing melt rates. In a region already affected by megadrought and shrinking snowpack, such albedo reductions threaten to further diminish freshwater availability. This study emphasizes the need to integrate local aerosol emissions—particularly from mining and transport activities—into hydrological and climate models for the Central Andes. The authors acknowledge the support of the National Research and Development Agency of Chile (ANID), namely, ANID-FONDECYT 3230555, ANID-FONDECYT 11220482, ANID-FONDECYT 11220525, ANID Vinculación Internacional FOVI240088, and ANID FONDEQUIP EQM250078, as well as the Multidisciplinary Research Project PI_M_24_03 from Universidad Técnica Federico Santa Maria (Chile). The spectroradiometric system was funded by the Spanish Ministry of Science and Innovation through the Acquisition of Scientific-Technique Equipment (2019) grant (ref. EQC2019-006105-P).

How to cite: Bolaño-Ortiz, T. R., McCracken, F., Ruggeri, M. F., Castro, L., González-Faune, L. A., Neira Román, J. A., Tovar-Bernal, F. A., and Lapuerta, M.: Experimental Reduction of Snow Surface Albedo by Local Black Carbon and Mineral Dust Deposition in the Andes of Laguna del Maule, Chile, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17638, https://doi.org/10.5194/egusphere-egu26-17638, 2026.

EGU26-18048 | ECS | Posters on site | CR7.3

Experimental assessment of different mineral dust on snow properties and melt dynamics under cold laboratory conditions 

Javier Bandrés, Eric Sproles, Jorge Pey, Xavier Querol, Carlos Pérez García-Pando, and Juan Ignacio López-Moreno

Understanding the role of mineral dust deposition on snow-covered surfaces is essential for improving predictions of snowmelt timing and magnitude in mountain and polar regions. This is particularly relevant given the global diversity of dust sources, such as North Africa and Central Asia, or regional sources related to human activities. While the radiative forcing of light-absorbing impurities is increasingly well documented, there is still limited understanding of how distinct mineral dust types and their associated mineralogical and geochemical compositions differently affect snowpack energy balance and melt processes. This knowledge gap persists because many models still assume a globally uniform mineralogical composition, leading to substantial uncertainties.

In this study, we present a series of controlled experiments conducted in the SubZero cold laboratories at Montana State University, using mini-lysimeters filled with snow artificially doped with varying and environmentally realistic concentrations of mineral dust samples originating from four distinct source regions (North Africa, Iceland, North America and the Middle East) under controlled environmental conditions in the cold chamber.

Our results suggest that Fe content is a key driver of the variability observed in snow darkening and melt enhancement. Dust-emitting sediments from the studied regions display distinct mineralogical compositions, with Fe contents varying 3.0 wt% in U.S. desert samples, 3.6 wt% in Moroccan dust, 5.5 wt% in mixed African dust sources, and substantially higher levels in Icelandic surface sediments, reaching up to 9.5 wt%.

Across experiments, the results show clear reductions in snow albedo, changes in specific surface area (SSA), and increases in liquid water content (LWC) and meltwater production for different dust types samples and concentrations.

The first author has an FPI predoctoral grant in the frame of MARGISNOW project (PID2021-124220OB-100) funded by the Spanish Ministry of Science and Innovation. This research received support from SNOWDUST (AEI, TED2021-130114B-I00), POSAHPI-2 (PID2022-143146OB-I00) and FRAGMENT (ERC-2017-COG, Grant agreement ID: 773051).

How to cite: Bandrés, J., Sproles, E., Pey, J., Querol, X., Pérez García-Pando, C., and López-Moreno, J. I.: Experimental assessment of different mineral dust on snow properties and melt dynamics under cold laboratory conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18048, https://doi.org/10.5194/egusphere-egu26-18048, 2026.

EGU26-18685 | ECS | Orals | CR7.3

Centennial Changes in Microclimate and Surface Mass Balance: A West Greenland Case Study 

Florina Roana Schalamon, Sebastian Scher, Andreas Trügler, Wolfgang Schöner, and Jakob Abermann

The local microclimate is both a key driver and in turn impacted by glacier wastage. Such feedbacks become particularly relevant in rapidly changing regions such as for West Greenland, where e.g. Qaamarujup Sermia has retreated by approximately 2 km between 1930/31 and 2022. This is the site where Alfred Wegener’s last expedition took place and where its members conducted pioneering glaciological and meteorological studies . Starting in 2022, we re-established a spatially distributed monitoring network extending from the coastline to the upper glacier, including automated weather stations, distributed air-temperature and humidity sensors, and surface mass-balance stakes. These observations allow us to investigate how a significant increase in the extent of ice-free valley surfaces caused by glacier retreat influences altitudinal temperature profiles and, ultimately, glacier melt.
Cluster analyses of temperature gradients reveal that the often-assumed environmental lapse rate of −6.5 K per kilometer only applies under certain conditions. In several cases, lapse rates differ markedly between the ice-free valley and the air above the glacier and show complex patterns. We investigate how these patterns are linked to synoptic forcing and cloud conditions, which control the depth and persistence of temperature inversions. 
To quantify the implications of these microclimatic structures for glacier melt, we combine the atmospheric observations with high-resolution melt measurements from automated and conventional mass-balance stakes. We find that in recent years, higher melt rates occur under the same air temperature departure as they did in the 1930s.  Sparse snow observations indicate that snow accumulation in 1930/31, with a maximum snow height of approximately 2 m, was higher than in the years since 2022, but remains within the range of extreme snow amounts as for instance represented in the CARRA reanalysis period (1991-2024).
Together, our results demonstrate that ongoing glacier retreat at Qaamarujup Sermia not only responds to atmospheric forcing but can actively reshape the local microclimate, leading to increasingly effective melt processes. These feedbacks are critical for understanding future mass-balance evolution of glaciers in a changing climate. 

How to cite: Schalamon, F. R., Scher, S., Trügler, A., Schöner, W., and Abermann, J.: Centennial Changes in Microclimate and Surface Mass Balance: A West Greenland Case Study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18685, https://doi.org/10.5194/egusphere-egu26-18685, 2026.

EGU26-19610 | ECS | Posters on site | CR7.3

Climate indices change during 21st century in high-resolution RCMs 

Anastasiia Chyhareva, Svitlana Krakovska, Liudmyla Palamarchuk, Marte Hofsteenge, Clara Lambin, José Abraham Torres Alavez, and Ruth Mottram

The Antarctic is a critical component of the global atmosphere-ocean-cryosphere interaction and is simultaneously one of the regions most sensitive to climate change. However, the response to climate change varies significantly across the continent. Therefore, it is crucial to understand how the Antarctic will be impacted by climate change during the 21st century.

The aim of the study is to define general features of climate change in the Antarctic based on climate indices simulated by  regional climate models (RCMs). We used WCRP standard climate indices: frost days (number of days with a daily minimum temperature  < 0°C),  ice days (number of days with a maximum temperature < 0°C), total annual precipitation, longest consecutive wet spell (number of consecutive days with >1 mm/day), longest dry spell (number of consecutive dry days <1 mm/day), simple precipitation intensity (annual precipitation divided by wet days), intense, heavy and extreme precipitation for the daily precipitation amounts (90th, 95th and 99th percentiles respectively). Indices were computed from three RCMs (HCLIM, MAR, RACMO) under the two storylines: (1) strong sea ice decrease and weak strengthening of the southern polar vortex; (2) weak sea ice loss but strong polar vortex strengthening. Results were compared across three periods: 1986–2005 (historical), 2041–2060 (mid-century), and 2081–2100 (end-of-century). Models results and further postprocessing were performed under Horizont2020 PolarRES and OCEAN ICE Projects.

A comparison of climatic indices from historical to the end of the century reveals a significant transition toward a warmer and wetter climate. These changes are most pronounced in the coastal regions and the Antarctic Peninsula, while the high-elevation interior remains relatively stable. Dramatic reduction in 'Ice Days' particularly on the Peninsula is projected. This reduction implies a substantial increase in surface melt potential and an extended thaw season, accompanied by a corresponding—though less severe—decrease in 'Frost Days'.

Simultaneously, the models project a clear increase in total annual precipitation, primarily over the Southern Ocean and coastal zones. Precipitation characteristics also shift, exhibiting increased daily intensity and a modest decrease in the length of 'Consecutive Dry Days' over the continental interior.

Precipitation extremes (99 th percentile) are heavily concentrated along the Antarctic Peninsula and coastal West Antarctica. In regions with significant orographic enhancement, localized intensities exceed 100 mm/day, whereas the interior plateau remains much less (<10 mm/day). 

Overall, both storylines illustrate a fundamental shift in the Antarctic climate during the 21st century—particularly in coastal zones—characterized by a longer, more intense melt season and hydrological cycle. These changes hold significant implications for ice shelf stability and overall ice-sheet mass balance.

How to cite: Chyhareva, A., Krakovska, S., Palamarchuk, L., Hofsteenge, M., Lambin, C., Torres Alavez, J. A., and Mottram, R.: Climate indices change during 21st century in high-resolution RCMs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19610, https://doi.org/10.5194/egusphere-egu26-19610, 2026.

EGU26-20553 | ECS | Orals | CR7.3

How Changes in Relative Humidity in the Polar Boundary Layer impact Arctic Amplification in Climate Models 

Sophia Wüsteney, Andreas Platis, Jens Bange, and Felix Pithan

The Arctic is warming three to four times faster than the global average due to multiple feedback processes – a phenomenon known as Arctic Amplification. Cloud feedbacks, in particular, represent one of the largest sources of uncertainty in projections of this amplified warming. Relative humidity (RH) is critical to these cloud feedbacks through its influence on cloud formation and radiation balance, yet changes in Arctic RH under a warming climate remain poorly understood.

Using 27 CMIP6 Coupled Model Intercomparison Project (CMIP6) models, this study investigates Arctic RH changes and their drivers by comparing historical conditions (1985-2015) with future projections under SSP5-8.5 (2070-2100). The multi-model mean reveals a robust vertical dipole pattern in surface-temperature-normalized RH changes across the Arctic. Near the surface (1000-925 hPa), RH decreases by up to 2 % K−1 in winter, while mid-tropospheric RH (950-750 hPa) increases. This counterintuitive pattern – surface drying despite increased open ocean from sea-ice loss – is particularly pronounced during autumn and winter. The dipole signal is strongest over regions experiencing substantial sea ice loss, but remains visible at reduced amplitude over persistent ice regions, indicating both local (sea-ice driven) and broader (stability-driven) components to the RH response.


The multi-model mean, however, emerges from markedly different individual model responses. DIPOLE models reproduce the characteristic dipole pattern with drying near the surface and moistening around 1 km above the surface; DECREASE models show drying in both layers; INCREASE models show moistening at both levels. While DIPOLE and DECREASE models both exhibit a dipole pattern over ice-loss regions, INCREASE models do not, suggesting fundamental differences in model physics that are also evident in present-day RH distributions. Cloud liquid and ice water changes do not follow the dipole pattern but instead show increases across all groups, with inter-group differences in magnitude and vertical extent. Cloud liquid water increases peak near 925 hPa in all groups but are strongest over ice-loss regions in DECREASE and DIPOLE models, while DIPOLE models show strong cloud ice increases throughout the lower troposphere (surface–700 hPa), INCREASE and DECREASE models exhibit two distinct maxima at 850 and 500 hPa.


The primary driver of the dipole pattern is the transition from a predominantly stable atmosphere over sea ice (with an RH maximum near the surface) to a well-mixed atmosphere over open ocean (with an RH maximum at cloud base). This physical mechanism suggests that the DIPOLE models have a more realistic representation of moisture in the Arctic boundary layer and its response to sea-ice loss. If further analysis can rule out the behaviour of the INCREASE and DECREASE models, we expect that this will allow us to better constrain Arctic cloud feedbacks.

How to cite: Wüsteney, S., Platis, A., Bange, J., and Pithan, F.: How Changes in Relative Humidity in the Polar Boundary Layer impact Arctic Amplification in Climate Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20553, https://doi.org/10.5194/egusphere-egu26-20553, 2026.

EGU26-20625 | ECS | Posters on site | CR7.3

Effect of Increasing freezing point Sea Ice Albedo, on controlling Arctic Climate variables in ICON 

Josien Rompelberg, Dörthe Handorf, Christoph Jacobi, and Evelyn Jäkel

Climate models have difficulties accurately representing Arctic mid-latitude linkages. This might partly be caused by surface parametrizations that are not able to accurately represent the Arctic surface conditions. As a result, large uncertainties arise in the modelling of energy exchange between the surface and the atmosphere, since sea ice surface albedo (SIA) controls the energy input in the Arctic region. The present study aims to gain insights in how the SIA parameterization scheme in the Icosahedral Nonhydrostatic (ICON) model can influence Arctic climate.

In order to identify the sources of error in the current SIA parameterization scheme, it is evaluated against Arctic observational data. The data includes both on-ice measurements to capture the SIA temporal evolution (MOSAiC), as well as airborne measurements from several flight campaigns performed within the (AC)3 project to capture a larger spatial variability. The offline evaluation, in which the SIA parametrization is isolated from the ICON model and observations are used as input for the parametrization, shows that the biggest disagreement between the scheme and the observations occurs at freezing point temperatures.  

Inspired by this outcome and to better understand how SIA parametrization can control the Arctic climate, a simulation with increased SIA at freezing point temperatures is performed. With this long term, limited area, pan-arctic simulation, changes in energy exchange between surface and atmosphere are analyzed. 

This work was supported by the DFG funded Transregio-project TRR 172 “Arctic Amplification (AC)3“.

How to cite: Rompelberg, J., Handorf, D., Jacobi, C., and Jäkel, E.: Effect of Increasing freezing point Sea Ice Albedo, on controlling Arctic Climate variables in ICON, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20625, https://doi.org/10.5194/egusphere-egu26-20625, 2026.

EGU26-22142 | ECS | Posters on site | CR7.3

Assessment of Circulation Weather Types around Svalbard and their Impact on the Ny-Ålesund Atmospheric Column 

Phillip Eisenhuth and Sandro Dahlke

Meteorological conditions in Ny-Ålesund (NYA), Svalbard, are influenced by the large-scale atmospheric circulation patterns, such as southerly or northerly advection as well as cyclonic or anticyclonic circulation regimes. We classify the prevailing synoptic circulation into a number of recurrent circulation weather types (CWT), to quantify their influence on local atmospheric column properties and their contribution to the observed Arctic amplification in NYA.

We construct a 45+ year CWT catalogue for NYA based on hourly 850 hPa geopotential fields from ERA5 reanalysis data using a modified Jenkinson-Collison classification. This catalogue is combined with long-term observational records from the AWIPEV radiosonde programme and the Baseline Surface Radiation Network (BSRN) in NYA.

Composite analyses reveal a pronounced directional and seasonal dependence of near-surface temperature, longwave net radiation and humidity on the prevailing CWT. Trends in CWT frequency indicate an increased occurrence of southerly advection in winter and autumn, which contributes to the enhanced warming in NYA in these seasons. Conversely, a higher frequency of northerly CWT in spring is associated with the observed cooling, particularly in March.

Consequently, CWT analysis and their long-term trends quantify the influence of synoptic circulation to atmospheric conditions in NYA and contribute to the explanation of the observed seasonal changes in the Svalbard region.

 

This work was supported by the DFG funded Transregio-project TRR 172 “Arctic Amplification (AC)3“.

How to cite: Eisenhuth, P. and Dahlke, S.: Assessment of Circulation Weather Types around Svalbard and their Impact on the Ny-Ålesund Atmospheric Column, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22142, https://doi.org/10.5194/egusphere-egu26-22142, 2026.

EGU26-2657 | Posters on site | CL4.13

Enhancing Coastal Hazard Projections in Singapore: Application of Bias Correction Techniques for Monsoon and Storm Surge Modeling 

Farzin Samsami, Pavel Tkalich, Sumit Dandapat, and Haihua Xu

Accurate modelling of monsoon and storm surge heights is crucial for effective coastal and climate resilience management in Singapore. Despite advances in climate modeling and hydrodynamic simulations, systematic biases remain a challenge, often resulting in under- or overestimation of extreme events and coastal hazards. Bias correction is crucial to improve the accuracy of projections. This study explores the application of several bias-adjustment techniques—mean bias correction, variance scaling, and quantile mapping—to improve the accuracy of monsoon and storm surge projections along Singapore’s coastlines. Mean bias correction adjusts the model output to match the observed mean better, whereas variance scaling further refines the distribution by adjusting the model output variance to match the observed variance. Quantile mapping provides a comprehensive approach by modifying the entire distribution of model outputs to match the observed distribution, creating a mapping between the model's Cumulative Distribution Function (CDF) and the observed CDF, which improves the simulation of both median and extreme values. In this study, outputs from the Delft3D FM hydrodynamic model, driven by atmospheric forcings from the Singapore Variable Resolution – Regional Climate Model (SINGV-RCM), which employs six global climate models (GCMs) from the CMIP6 climate projections, were compared with observed data at multiple tide gauge stations in the region. We applied these bias-correction methods individually to historical simulations (1984-2014) and in combination to project future monsoon and storm surge heights (2015-2100). The corrected projections are evaluated through statistical metrics and comparison with historical observations, demonstrating significant improvements in model accuracy and reliability. Our results highlight that quantile mapping provides the most comprehensive bias correction, capturing the full distribution of extreme events, while mean bias correction and variance scaling offer simpler, computationally efficient alternatives.

How to cite: Samsami, F., Tkalich, P., Dandapat, S., and Xu, H.: Enhancing Coastal Hazard Projections in Singapore: Application of Bias Correction Techniques for Monsoon and Storm Surge Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2657, https://doi.org/10.5194/egusphere-egu26-2657, 2026.

EGU26-3382 | ECS | Posters on site | CL4.13

Documenting the transition from late Holocene relative sea-level fall to observed modern rise in Vesterålen, Northern Norway 

Oskar Eide Lilienthal, Kristian Vasskog, and Francis Chantel Nixon

Most of the outer Norwegian arctic coastline is experiencing relative sea-level (RSL) rise despite being near-field areas with ongoing vertical land uplift due to glacioisostatic adjustment. However, due to a lack of pre-instrumental RSL-data over the last millennium, the transition from falling to rising RSL is not well constrained in time and space.

In this project we have reconstructed the past 500 years of RSL-history of the Vesterålen archipelago in northern Norway. We have analyzed salt-marsh sediments using preserved agglutinated foraminifera as proxy evidence of local RSL- change. Our data bridges the gap between the instrumental record and previous palaeo-RSL reconstructions and provides new insights into the recent sea-level history of the region.

Here, we will present our modeled RSL-curve and highlight our main results regarding when the transition from sea-level regression to the current sea-level transgression occurred, and the magnitude of post-industrial sea-level rise in the region.

How to cite: Lilienthal, O. E., Vasskog, K., and Nixon, F. C.: Documenting the transition from late Holocene relative sea-level fall to observed modern rise in Vesterålen, Northern Norway, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3382, https://doi.org/10.5194/egusphere-egu26-3382, 2026.

EGU26-3396 | Orals | CL4.13

Evidence of increased deep ocean warming from a sea level budget approach 

Anny Cazenave, Chunxue Yang, Marie Bouih, Andrea Storto, Jianli Chen, William Llovel, Karina von Schuckmann, and Lancelot Leclercq

Assessments of the global mean sea level (GMSL) budget over the satellite altimetry era (since the early 1990s) have concluded that the GMSL budget is closed within data uncertainties until 2016. However, studies have shown that since then, the sea level budget based on Argo data down to 2000 for the thermosteric contribution is no longer closed. Using an ocean reanalysis with no altimetry data assimilation, we show that accounting for deep ocean thermosteric contribution (below 2000 m, not sampled by Argo) allows the GMSL budget to be almost closed since 2016. The deep ocean contribution over 2005-2022 is estimated to 0.4 ± 0.15 mm/yr, i.e., about 10%. to the observed GMSL rise over that period. This finding reveals that deep ocean warming is gaining importance and that ocean heat uptake has now reached several regions below 2000m depth, notably the Northwestern Atlantic Ocean and areas around Antarctica.

 

How to cite: Cazenave, A., Yang, C., Bouih, M., Storto, A., Chen, J., Llovel, W., von Schuckmann, K., and Leclercq, L.: Evidence of increased deep ocean warming from a sea level budget approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3396, https://doi.org/10.5194/egusphere-egu26-3396, 2026.

EGU26-3430 | ECS | Orals | CL4.13

Abrupt trend change in global mean sea level and its components in the early 2010s 

Lancelot Leclercq, Julius Oelsmann, Anny Cazenave, Marcello Passaro, Svetlana Jevrejeva, Sarah Connors, Jean-François Legeais, Florence Birol, and Rodrigo Abarca-del-Río

Abrupt changes at decadal time scale are recurrent events in the modern climate system. Using multiple trend-change detection methods, here we report such an abrupt trend change in the early 2010s in the altimetry-based global mean sea level record, as well as in its thermal and mass components. Abrupt trend change in the mass component is mostly due to terrestrial water storage and to a lesser extent to ice sheet melting. The linear rate of rise of the global mean sea level increases abruptly from 2.9 ± 0.22 mm yr-1 over 1993-2011 to 4.1 ± 0.25 mm yr-1 over 2012-2024. Abrupt trend changes in numerous climate parameters have also been reported in the early 2010s, suggesting a more global phenomenon. Internal climate variability is likely the main driver of the early 2010s sharp change observed in sea level and components, although one cannot totally exclude any additional contribution from increased radiative forcing.

How to cite: Leclercq, L., Oelsmann, J., Cazenave, A., Passaro, M., Jevrejeva, S., Connors, S., Legeais, J.-F., Birol, F., and Abarca-del-Río, R.: Abrupt trend change in global mean sea level and its components in the early 2010s, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3430, https://doi.org/10.5194/egusphere-egu26-3430, 2026.

EGU26-4116 | ECS | Posters on site | CL4.13

 Intrinsic ocean variability partly randomizes the mean seasonal cycle of sea level  

Carmine Donatelli, Rui M. Ponte, Thierry Penduff, Mengnan Zhao, and William Llovel

Oceanic nonlinearities drive random intrinsic sea level variations over the global ocean, which locally compete with forced sea level variations that are paced by atmospheric and astronomical drivers. This study utilizes a global ocean/sea-ice 50-member ensemble simulation to characterize the sea level mean seasonal cycle (computed over 1993-2015) and partition its forced and intrinsic components. The model faithfully represents many features of the observed sea level mean seasonal cycle. We show that the mean seasonal cycle of sea level is most stochastic in the Southern Ocean, in western boundary currents, and along +/-20° latitudes, and remains partly random up to 10°x10° scales in these regions. Forced and intrinsic components mostly have a steric origin but with deeper signals involved for the intrinsic term. Our study thus demonstrates that ocean nonlinearities give a marked stochastic flavor to the sea level seasonal cycle averaged over 23 years and illustrates the usefulness of eddying ocean ensemble simulations for adequately interpreting observations.

How to cite: Donatelli, C., Ponte, R. M., Penduff, T., Zhao, M., and Llovel, W.:  Intrinsic ocean variability partly randomizes the mean seasonal cycle of sea level , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4116, https://doi.org/10.5194/egusphere-egu26-4116, 2026.

The Southern Ocean (SO) plays a crucial role in the global climate system by absorbing heat and carbon dioxide from the atmosphere. Understanding sea level changes and associated physical processes in the SO can provide valuable insights into how the ocean contributes to regulating Earth’s climate. Ocean dynamical processes are crucial for redistributing ocean heat and mass, thereby significantly influencing sea level change in the SO and globally. Here we investigate the mechanisms of thermal and ocean mass (ocean bottom pressure, OBP) variations, which are two important components of sea level variability. Observations show that since the 1950s, the subsurface South Hemishphere has been rapidly warming in the south and cooling in the north. A theoretical analysis and ocean model perturbation experiments indicates that the subsurface cooling is mainly attributed to pure heaving caused by wind stress change. In the SO, OBP variations explain most of large-scale sea level variations at seasonal-to-decadal time scales. Regional OBP variations are mainly driven by surface wind and regulated by the bottom topography. Strong OBP signals are located in the deep basins where closed planetary vorticity isolines present. At interannual time scales, OBP patterns in the SO are closely associated with El Niño-Southern Oscillation and Southern Annular Mode, which can indicate interannual variability of Antarctic Circumpolar Current transport to a great extent.

How to cite: Cheng, X.: Ocean dynamical processes underlying sea-level change and variabilityin the Southern Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4577, https://doi.org/10.5194/egusphere-egu26-4577, 2026.

EGU26-6033 | ECS | Posters on site | CL4.13

Near-term future sea-level projections supported by extrapolation of tide-gauge observations 

Jinping Wang, Xuebin Zhang, John Church, Matt King, and Xianyao Chen

Global, regional and local sea-level projections rely on complex process-based models of the climate-ocean-cryosphere system. While extrapolation of observational data has been examined on global and regional scales, this approach has not yet been used for the additional complexities of coastal sea-level projections. Here, we evaluate the sea-level trend and acceleration for a global network of 222 tide-gauge observations over 1970-2023, which are then extrapolated to provide local projections up to 2050 and compared with the process-based projections from the IPCC AR6. For 2050 relative to 2020, the observation-based and medium-confidence AR6 projections agree within the likely range at 96% of tide-gauge locations. Despite larger spatial variability, the observation-based projections are usually well below the low-likelihood, high-impact AR6 projections. The observation-based projections provide complementary perspectives of near-term local sea-level changes, and this agreement provides increased confidence in the current understanding and projections of sea-level changes over coming decades.

How to cite: Wang, J., Zhang, X., Church, J., King, M., and Chen, X.: Near-term future sea-level projections supported by extrapolation of tide-gauge observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6033, https://doi.org/10.5194/egusphere-egu26-6033, 2026.

The world’s coasts face the increasing risk of relative sea-level rise due to climate-induced sea-level rise and negative vertical land motion (i.e. land subsidence).  The impacts of relative sea-level rise and coastal (and compound) flooding are closely related to the land’s elevation relative to sea level. Consequently, the reliability of relative sea-level rise impact and flood exposure assessment heavily relies on the correct alignment of land elevation data and sea-level information. However, this is often not the case.

Based on a systematic evaluation of the scientific literature (385 studies), we found that over 90% of contemporary sea-level rise and coastal hazard impact assessments do not apply sea-level information in addition to land elevation data and therefore fail to properly align land elevation to observed coastal sea level. From the 10% of the assessments that combined sea-level and land elevation data, 9% contain incomplete methodological documentation (rendering the study irreproducible) and/or contain flaws in vertical datum conversion and dataset combination. Less than 1% properly align sea level and land elevation and provide full methodological documentation. Our meta-analyses revealed sea-level height to be globally on average 0.3 m higher than commonly assumed, with a disproportionate impact on the Global South and differences of more than 1 m in most affected regions in the Indo-Pacific. This translates into worldwide 37% more land and up to 68% more people exposed to a 1 m relative sea-level rise. As many of the reviewed studies inform policy reports (e.g. IPCC reports), the widespread underestimation of coastal exposure may have far-reaching implications for policymaking and coastal adaptation.

Our findings reveal a community-wide methodological blind spot which calls for systemic, cross-disciplinary changes. To overcome the methodological challenges to properly align coastal land and sea-level information and prevent future errors, we provide properly combined coastal elevation information referenced to local sea level. To ensure proper data integration and reproducibility of coastal impact assessments, we also recommend to introduce author declarations and review checklists into the scientific peer-review process. These actions will raise community-wide awareness on the current blind spot, prevent future error propagation and improve transparency and reproducibility of impact studies. This will lead to improved future sea-level rise and other coastal hazard assessments and strengthen the scientific information available for policy-informing reports, like the upcoming IPCC AR7 reports.

How to cite: Seeger, K. and Minderhoud, P.: Coastal sea level higher than assumed in most sea-level rise impact assessments: Revealing a methodological blind spot, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6244, https://doi.org/10.5194/egusphere-egu26-6244, 2026.

EGU26-6572 | Posters on site | CL4.13

Long-term Prediction of Sea-Level Changes around the Korean Peninsula over the Next One Million Years using a Conceptual Global Sea-Level Model 

Joo-Hong Kim, Sang-Yoon Jun, Taewook Park, Wonsun Park, Keyhong Park, Yeongcheol Han, Kwangchul Jang, and Changhee Han

This study presents long-term projections of global and regional sea level changes over the next one million years using a conceptual global sea level model, and evaluates the corresponding shoreline variations around the Korean Peninsula. The global ice-volume variations over the past one million years were first simulated using a conceptual global ice-volume model, and the modeled results show a strong correlation with proxy-based global sea level reconstructions, with correlation coefficients of –0.78 for the past 800 kyr and –0.81 for the past 500 kyr, confirming the model’s long-term reproducibility. Future simulations applying five Shared Socioeconomic Pathway (SSP) greenhouse gas scenarios indicate that under low-emission scenarios (SSP1–2.6 and SSP2–4.5), the next glacial inception is expected to occur approximately 50–60 kyr from the present. In contrast, under high-emission scenarios (SSP3–7.0 and SSP5–8.5), the onset of the next glaciation is delayed until 120–170 kyr in the future. Notably, the SSP5–8.5 scenario projects an exceptionally prolonged interglacial period lasting over 100 kyr, with a global mean sea-level rise of up to 24 m that persists for an extended duration. Based on these results, the future shoreline configurations around the Korean Peninsula were reconstructed. Depending on the scenario, global sea level is projected to rise by approximately 12–21 m within the next millennium, resulting in a marked inland retreat of coastlines, particularly along the western and southern coasts of Korea, including the Hwanghae and Chungcheong regions. After 50 kyr, certain scenarios show coastal expansion due to sea-level fall, while after 100 kyr, the progression toward the next glacial maximum leads to a complete exposure of the Yellow Sea basin.

How to cite: Kim, J.-H., Jun, S.-Y., Park, T., Park, W., Park, K., Han, Y., Jang, K., and Han, C.: Long-term Prediction of Sea-Level Changes around the Korean Peninsula over the Next One Million Years using a Conceptual Global Sea-Level Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6572, https://doi.org/10.5194/egusphere-egu26-6572, 2026.

EGU26-6946 | Posters on site | CL4.13

Assessing emulated multi-century global mean sea level projections - the Sea Level Emulator Intercomparison Project (SLEIP) 

Alexander Nauels, Tessa Möller, Victor Couplet, Robert E. Kopp, Praveen Kumar, Matthias Mengel, Gregory Munday, Zebedee R. J. Nicholls, Matthew D. Palmer, Lennart Ramme, Aimée B. A. Slangen, Chris Smith, Jennifer H. Weeks, and Tony E. Wong

Simplified sea level modelling approaches are developed to efficiently explore future sea level rise and associated uncertainties. Sea level emulators (SLEs) are mostly calibrated against the responses of process-based complex models, they can be run on multi-century timescales and feed into regionalisation efforts, integrated assessment and coastal risk modelling. Here, we introduce the Sea Level Emulator Intercomparison Project (SLEIP) to systematically assess available sea level emulators and identify future research needs to maximise the utility of this modelling approach. SLEIP covers 13 datasets from the participating models BRICK (with DOECLIM and SNEASY climate forcing), FACTS (7 individual emulator workflows), FRISIA, MAGICC, ProFSea and SURFER. All of the participating SLEs produce projections out to the year 2300 for the main sea level drivers thermal expansion, glacier mass loss, Greenland and Antarctic ice sheet mass loss, and land water storage. Participating SLEs differ in whether and how they account for low-confidence, high-impact processes of poorly known likelihood, such as marine ice-cliff instability (MICI). The SLE components with the largest response range are the Greenland and Antarctic ice sheet, with the Antarctic ice sheet becoming the most uncertain sea level driver in 2300. With identical MAGICC climate forcing input, 2300 median global mean sea level rise estimates range from 0.46 m to 1.71 m (outer 17th-83rd percentile range: 0.32-3.20 m) under very low emissions (SSP1-1.9), 0.67 m to 2.01 m (0.47-3.56 m) under low emissions (SSP1-2.6), 1.64 m to 4.07 m (1.15-10.53 m) under moderate emissions (SSP2-4.5), 2.35 m to 9.33 m (1.68-14.39 m) under high emissions (SSP3-7.0), and 2.44 m to 11.16 m (1.74-15.79 m) under very high emissions (SSP5-8.5), all relative to 1995-2014. SLEIP also allows investigating the sea level response under overshoot. Under the overshoot scenario SSP5-3.4-OS (peak GMT: 2.3 °C, 2100 GMT: 1.9 °C), median projections range from 0.45 m to 0.86 m (0.36-1.31 m) in 2100 and 0.80 m to 2.30 m (0.56-9.82 m) in 2300.

How to cite: Nauels, A., Möller, T., Couplet, V., Kopp, R. E., Kumar, P., Mengel, M., Munday, G., Nicholls, Z. R. J., Palmer, M. D., Ramme, L., Slangen, A. B. A., Smith, C., Weeks, J. H., and Wong, T. E.: Assessing emulated multi-century global mean sea level projections - the Sea Level Emulator Intercomparison Project (SLEIP), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6946, https://doi.org/10.5194/egusphere-egu26-6946, 2026.

EGU26-8862 | Posters on site | CL4.13

Multi-Decadal Sea Level Rise along the Korean Coasts Based on L2-Quality Reprocessed Tide Gauge Observations 

Kwang-Young Jeong, Haejin Kim, Hyunsik Ham, Hwa-Young Lee, Bon-Ho Gu, Gwang-Ho Seo, and Yang-Ki Cho

Sea level rise is a key indicator of climate change and a major driver of coastal flooding and erosion. Reliable assessment of long-term sea level trends requires high-quality, internally consistent observations that account for instrumental changes and vertical land motion. In this study, we present the reprocessing of long-term tide gauge records around the Korean Peninsula to generate Level-2 (L2) delayed-mode sea level height data and assess recent multi-decadal sea level rise from a climate change perspective. Historical tide gauge observations from 21 coastal stations were reprocessed from the beginning of measurements to December 2024 using a comprehensive quality control framework. The reprocessing procedure includes station history investigation, residual comparison, relative sea level difference analysis with neighboring stations, and scientific interpolation of missing or abnormal data. To accurately quantify long-term sea level variability, vertical land motion associated with coastal structures and ground subsidence was evaluated using precise leveling surveys, GNSS-derived vertical displacement, and satellite-based SAR imagery, and applied as corrections to the sea level records. As a result, consistent hourly L2-quality sea level datasets with observation periods exceeding 30 years were reconstructed. Using the reprocessed datasets, sea level rise rates along the Korean coast were estimated. Over the past 36 years, mean sea level has risen at an average rate of 3.17 mm yr⁻¹, corresponding to an increase of approximately 11.5 cm. Regional variability is evident: rise rates of 3.06–3.6 mm yr⁻¹ are observed along the west and east coasts, while the south coast exhibits relatively lower rates of 2.6–3.4 mm yr⁻¹. Decadal analysis for the last 30 years (1995–2004, 2005–2014, and 2015–2024) reveals temporal and regional variations in sea level rise, with periods of acceleration and deceleration depending on coastal region. The reconstructed L2 sea level datasets provide a robust observational basis for climate change assessment, coastal hazard analysis, and ocean–climate interaction studies. The L2 data will be publicly released via the Korea Hydrographic and Oceanographic Agency in the first half of this year, supporting reproducible and policy-relevant sea level research.

How to cite: Jeong, K.-Y., Kim, H., Ham, H., Lee, H.-Y., Gu, B.-H., Seo, G.-H., and Cho, Y.-K.: Multi-Decadal Sea Level Rise along the Korean Coasts Based on L2-Quality Reprocessed Tide Gauge Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8862, https://doi.org/10.5194/egusphere-egu26-8862, 2026.

EGU26-10322 | ECS | Orals | CL4.13

Feedback-based sea level rise impact modelling for integrated assessment models with FRISIAv1.0 

Lennart Ramme, Benjamin Blanz, Christopher Wells, Tony Wong, Cecilie Mauritzen, William Schoenberg, Chris Smith, and Chao Li

The socio-economic costs of sea level rise (SLR) are an important component of climate impact representations in integrated assessment models (IAMs). However, the representation of global or regional mean SLR and its impacts varies substantially between different IAMs; from no representation at all to the use of regionally resolved coastal impact models with more than 10,000 individual coastal segments. Current SLR impact models thereby often follow a cost-benefit analysis approach, might not represent diverse pathways of SLR impacts, or miss coastal adaptation. Especially, there is a lack of process-based models of SLR impacts with a focus on global, time-varying dynamics.

Here, we present a new modelling framework, the Feedback-based knowledge Repository for Integrated assessments of Sea level rise Impacts and Adaptation version 1.0 (FRISIAv1.0), a model designed for process-based, non-equilibrium IAMs. Its formulation for the calculation of global mean sea level rise is based on existing models, while its impact and adaptation component is a substantially modified derivation of the Coastal Impact and Adaptation Model (CIAM) for use in globally or regionally aggregated models. FRISIA follows a system dynamics approach, focusing on interconnectedness and feedback between components that is often missing in existing models. Examples of such additional connections included in FRISIA are: a reduction of local asset values and GDP per capita through the increasing storm surge damages, reduced investment in coastal zones under expected increases in exposure, and a limitation to the amount of money that can annually be spent on flood protection.

A version of FRISIA without these feedbacks approximately reproduces CIAM's results, while their integration leads to emerging new behaviour, such as a potential peak and decline in SLR-driven storm surge damages in the early 22nd century, due to economic feedbacks in the coastal zone. When coupling FRISIA to an IAM, global GDP is reduced by 1.5 - 6.2 % (17th - 83rd percentile range) under the mean SSP5-8.5 global-mean sea level rise from the IPCC's AR6 report (0.77 m by 2100) and no coastal adaptation, which is within the range reported in previous studies. We further show that the coupling of a diverse set of SLR impact streams into a process-based IAM allows the representation of a wide range of socio-economic consequences, such as effects on GDP, inflation, mortality or public debt.

As an outlook, we explore different adaptation strategies in a set of sensitivity simulations with FRISIA, focusing on the effect of delays and interruptions in flood protection investments on optimal SLR adaptation strategies. We find that both aspects can reduce the likelihood that a protect strategy (such as building a sea wall) is the optimal strategy, and we highlight the risk of a positive feedback loop of increasing SLR damage, reduced economic growth and reduced protection investments that might be triggered in some regions.

How to cite: Ramme, L., Blanz, B., Wells, C., Wong, T., Mauritzen, C., Schoenberg, W., Smith, C., and Li, C.: Feedback-based sea level rise impact modelling for integrated assessment models with FRISIAv1.0, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10322, https://doi.org/10.5194/egusphere-egu26-10322, 2026.

EGU26-10482 | ECS | Posters on site | CL4.13

The Impact of Delays and Interruptions on Optimal Sea-Level Rise Adaptation under Uncertainty 

Lennart Ramme, William Schoenberg, Benjamin Blanz, Cecilie Mauritzen, Christopher Wells, and Chao Li

Global warming leads to sea level rise (SLR), and coastal zones will have to adapt to avoid extensive impacts on people and capital. Possible adaptation strategies can be broadly categorized into no (only autonomous) adaptation, adaptation via retreat from the coast, and protection construction or other forms of accommodation to rising sea levels. Cost-benefit analysis often suggests retreat as the “optimal” strategy for the majority of the (rural) coastline, whereas protection is typically suggested for coastal zones with relatively high population or capital densities.

Here, we use the new FRISIA modelling tool to explore the effect that delays in adaptation and interruptions in flood protection investments can have on what the optimal SLR adaptation strategy is. We thereby define optimality not just by a single metric that combines several quantities, but look at monetary costs, people affected and flood fatalities separately, thereby offering more insights and avoiding the difficult weighting of people and capital.

Sensitivity experiments indicate that delaying the start year of adaptation via retreat or protection reduces the likelihood that protection is the optimal strategy in favour of retreat, especially when considering people rather than monetary impacts. This is mostly because protection construction takes longer and might be imperfect due to limitations in money availability in regions with low population and capital density.

Accounting for interruptions in flood protection investments reduces the likelihood that protection remains the optimal adaptation strategy, particularly in coastal zones that are close to the affordability threshold for building protection. We demonstrate that a reinforcing feedback loop, whereby increasing SLR-induced damage depresses economic growth and thereby places further constraints on protection investments, can be triggered in regions with low population and capital density. Our results further indicate a heightened risk of escalating damages in regions with intermediate population and capital density. In these areas, conventional cost–benefit analysis may still identify protection as the preferred strategy, yet this outcome is highly sensitive to interruptions or constraints in investment, rendering these regions especially vulnerable to adverse development pathways.

How to cite: Ramme, L., Schoenberg, W., Blanz, B., Mauritzen, C., Wells, C., and Li, C.: The Impact of Delays and Interruptions on Optimal Sea-Level Rise Adaptation under Uncertainty, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10482, https://doi.org/10.5194/egusphere-egu26-10482, 2026.

EGU26-11299 | ECS | Posters on site | CL4.13

Priorities in coastal protection due to extreme sea levels under sea level rise 

Christian Jordan, Torsten Schlurmann, Leon Scheiber, Nils Goseberg, and C. Gabriel David

Extreme sea levels (ESLs) pose severe flood risks to coastal communities. Climate change is amplifying these risks as sea level rise (SLR) will increase the probability of given baseline ESL events. This will challenge coastal design standards relying on fixed return periods, as this assumption becomes obsolete under rapidly changing climate conditions. This study evaluates how future SLR will transform ESL return periods and compress the windows for adaptation along the German Bight at the North Sea coast.

Using data from the coastDat-2 hindcast – a high-resolution dataset of water levels and waves for the North Sea region –  we performed statistical analyses to derive return curves for regional ESLs, linking return heights to their corresponding return periods. These return curves were then combined with sea level projections from the Sixth Assessment Report (AR6) of the Intergovernmental Panel on Climate Change (IPCC) under various global warming scenarios. From this integrated analysis, we calculated two key metrics: amplification factors (AFs) and timings. The AFs quantify how much more probable a baseline event will become under future SLR conditions, whereas the timings describe the available timeframe before a specific amplification threshold is exceeded, providing valuable information about windows for adaptation planning.

Our results demonstrate that AFs across the study region increase substantially with higher warming levels, dramatically raising the probability of baseline ESL events becoming commonplace. Timings also shrink considerably under rising temperatures, highlighting the accelerating urgency for proactive adaptation measures. Importantly, we also identified significant regional variability in how coastal locations respond to SLR. Locations with lower baseline ESL return heights – associated with smaller tidal ranges and lower water level variability – experience larger amplification sooner. At these sites, a 100-year ESL event could become a 10-year event (AF = 10) within only a few decades under high warming levels, whereas this threshold will be exceeded much later elsewhere. This spatial heterogeneity emphasizes that effective adaptation strategies must be tailored to the local response to SLR rather than applying uniform, coast-wide approaches.

For practical adaptation planning, AF thresholds can be translated directly into required intervention frequencies. Establishing widely accepted thresholds is crucial for implementation: lower AF thresholds better manage residual flood risk but compress adaptation windows, potentially necessitating a paradigm shift from occasional adjustments to continuous adaptation.

How to cite: Jordan, C., Schlurmann, T., Scheiber, L., Goseberg, N., and David, C. G.: Priorities in coastal protection due to extreme sea levels under sea level rise, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11299, https://doi.org/10.5194/egusphere-egu26-11299, 2026.

EGU26-13410 | Posters on site | CL4.13

Review of Sea-Level Budget Components and Their Consistency in the Recent Literature 

Valentina R. Barletta, Andrea Bordoni, and Shfaqat Abbas Khan

Closing the global sea-level budget is a central goal of climate research, as failing to do so could indicate that some components are not properly assessed. Yet achieving agreement between the measured total sea-level rise and the sum of its contributions does not necessarily reflect consistency among the individual components. In this study, we compile and compare published estimates from the past two decades for ice-sheet and glacier mass balance, land water storage, and steric expansion, and complement them with mass‑change trends from GRACE-derived products.

For each component, we find a substantial spread among published estimates, often larger than the reported uncertainties. These discrepancies persist even in reconciled or community-based products, particularly in regions with limited observational coverage and where different methodologies, models, or datasets are used. This is especially visible for land water storage and ice-sheet mass balance, and in the last decade also for steric expansion.

These findings suggest that the closure of the sea-level budget can mask compensating errors among its components. Rather than undermining confidence, the aim of our work is to identify where efforts should focus in order to reduce uncertainties and strengthen future assessments of global sea-level change.

How to cite: Barletta, V. R., Bordoni, A., and Khan, S. A.: Review of Sea-Level Budget Components and Their Consistency in the Recent Literature, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13410, https://doi.org/10.5194/egusphere-egu26-13410, 2026.

EGU26-13445 | ECS | Posters on site | CL4.13

Mediation of sea level from the open ocean to the coast 

Sam T. Diabaté, Neil Fraser, and Gerard McCarthy

Sea level is rising globally, threatening the world coastlines. In this context, it is of paramount importance to understand the physical mechanisms driving spatiotemporal coastal sea-level changes. The adaptation of the coastal sea level to seawater density changes in the open ocean remains, for example, rather poorly understood. The present talk is a contribution towards this understanding. In the flat-bottomed open ocean, density horizontal gradients yield alone the presence of geostrophic baroclinic circulation and spatial variations in steric sea level. At the margins of oceanic basins, the situation is very different. The presence of continental slopes is a vorticity barrier hindering baroclinic geostrophic transport towards the coast and accumulation or removal of water there. In addition, the steric sea level vanishes at the coast where the seafloor depth is zero. In the low-frequency limit, how coastal sea level can be impacted by open ocean density spatiotemporal changes is hence non-trivial and must involve ageostrophic mechanisms. Here, we show that seawater density gradients generate large along-slope currents because of the Joint Effect of Baroclinicity and Relief (JEBAR). The latter currents are slowed down by bottom friction, which in the process transmits the sea level – originally of open ocean and steric origin – to the coast as manometric changes. The framework used is the Arrested Topographic Wave theory extended to a baroclinic ocean.

How to cite: Diabaté, S. T., Fraser, N., and McCarthy, G.: Mediation of sea level from the open ocean to the coast, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13445, https://doi.org/10.5194/egusphere-egu26-13445, 2026.

EGU26-13655 | ECS | Orals | CL4.13

2023-2024 El Niño amplifies record sea level surges in African marine domains 

Franck Eitel Kemgang Ghomsi, Julienne Stroeve, Alex Crawford, Alain Tamoffo, Fernand Mouassom, and Moagabo Ragoasha

Africa's coastal regions, already burdened by accelerating sea level rise, faced unprecedented threats from the 2023–2024 El Niño, which triggered record surges across marine domains while compounding a long-term regional increase of 11.26 cm since 1993. Here we analyze high-resolution satellite altimetry from 1993 to 2024. Our analysis reveals how anomalous winds suppressed coastal upwelling, sparking marine heatwaves. This drove a record upper-ocean heat buildup, quadrupling prior maxima, and produced a regional surge of 8.39 cm. Steric effects accounted for over 80% of the rise in the Atlantic and Indian Oceans, with thermal expansion dominating the steric signal, while in the Mediterranean, ocean mass changes played a nearly equal role. Thermal expansion was the overwhelming driver, with steric effects accounting for over 80% of the rise in the Atlantic and Indian Oceans, while in the Mediterranean, ocean mass changes played a nearly equal role. Critically, this event’s disproportionate impact demonstrates nonlinear amplification. Record ocean stratification, more than double that of previous super El Niños, trapped surface heat, intensifying the steric response. This is magnified by a post-2008 regime shift that increased sea level trends by 71%. Consequently, El Niño events now explain 24.7% of interannual variability, underscoring their growing dominance. This dynamic creates a compound threat for Africa’s vulnerable coasts: extreme flood risks from sea level rise and land subsidence (>3 mm/year) are coupled with collapsing marine productivity, demanding urgent adaptation in low-lying deltas and Small Island Developing States.

How to cite: Kemgang Ghomsi, F. E., Stroeve, J., Crawford, A., Tamoffo, A., Mouassom, F., and Ragoasha, M.: 2023-2024 El Niño amplifies record sea level surges in African marine domains, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13655, https://doi.org/10.5194/egusphere-egu26-13655, 2026.

Coastal Louisiana, particularly the Mississippi River Delta region, faces some of the largest rates of relative sea-level rise worldwide (>9.3 mm/yr since 1947 at Grand Isle). These large rates are dominantly driven by (nonlinear) land subsidence, but larger-scale oceanic processes in the Gulf of Mexico and the adjacent North Atlantic have also contributed to these rates, particularly over the past ~15 years. In the past, relative sea-level rise in the region has usually been approximated by means of the Grand Isle tide gauge record even though it is well known that local processes, such as subsidence and hydrologically driven processes, can vary significantly locally. Here we introduce a set of thirty-one daily tide-gauge records maintained by the U.S. Army Corps of Engineers and located throughout southern Louisiana. However, there exist several inhomogeneities within these records, including undocumented datum shifts, which necessitated the development of a homogenization framework to properly analyze trends. Given the unique issues with the dataset, particularly the spatial isolation of some tide gauges, we develop a new approach using probabilistic principal component analysis to homogenize these records in place of the traditional buddy-checking approach. Significant spatial and temporal variability in long-term sea-level trends is found in these newly homogenized records. The Lower Mississippi Delta region (also known as the Birdsfoot) stands out with the largest long-term trends on the order of 35 mm/yr, more than three times the value obtained at Grand Isle and more than twenty times the value obtained from the global average. We identify subsidence as the main driver of these changes and provide new evidence that oil and gas withdrawals have significantly contributed to them.

How to cite: Hendricks, N. and Dangendorf, S.: Tide-Gauge Data Archaeology in Coastal Louisiana Reveals Relative Sea-Level Trends Up to Twenty Times the Global Average since 1950, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14501, https://doi.org/10.5194/egusphere-egu26-14501, 2026.

EGU26-17399 | Posters on site | CL4.13

Robust trends in Baltic sea level from satellite altimetry observations 

Susana Barbosa and Reik Donner

Regional sea-level change in the semi-enclosed Baltic Sea is strongly influenced by atmospheric forcing and wind-driven redistribution of water masses, leading to significant spatial variability in absolute sea level trends across the different sub-basins. This study focusses on absolute sea level trends in the Baltic Sea using satellite gridded sea level anomalies (0.0625º) from the European Seas Gridded L4 product provided by the E.U. Copernicus Marine Service (https://doi.org/10.48670/moi-00141). The daily time series (from January 1993 to the end of December 2023) are first deseasoned by removing the average annual cycle at each point. Then robust linear trends are estimated at each grid point by computing median slopes. In contrast to ordinary least-squares slopes characterising linear trends in the mean, these median slopes are calculated by minimising the mean absolute deviation of a linear trend model from the observations instead of the mean quadratic deviation, which makes them more robust to outliers and sensitive to the typical tendency of changes rather than to large deviations. Uncertainty is computed assuming non-independence by the Huber sandwich robust estimator for the covariance matrix.

The derived median slopes are in general higher than ordinary linear trends in the mean, except in the northern and easternmost areas of the Baltic. In the Bay of Bothnia ordinary linear trends and median trends are very similar, while in the eastern end of the Gulf of Finland median trends are similar or even slightly lower than ordinary linear trends. In the remaining areas, median trends are significantly larger than ordinary linear trends, the largest difference occurring in the Bothnian Sea. Coastal areas exhibit trends that differ from those in the adjacent basins. In the Gulf of Finland, median trends are higher than ordinary linear trends along the Finnish coast, whereas along the Roslagen coast (northern Stockholm Archipelago) the two slope estimates are in good agreement. Along the southern coastline of the Bothnian Sea, median sea-level trends reach the highest values, exceeding 6 mm/year.

The present study is financed within the scope of the Recovery and Resilience Mechanism (MRR) of the European Union (EU), framed in the Next Generation EU, for the period 2021 - 2026, within project NewSpacePortugal, with reference 11.

How to cite: Barbosa, S. and Donner, R.: Robust trends in Baltic sea level from satellite altimetry observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17399, https://doi.org/10.5194/egusphere-egu26-17399, 2026.

EGU26-18937 | ECS | Posters on site | CL4.13

Multi-century sea-level projections and human impacts under the indicative ScenarioMIP-CMIP7 forcings 

Jennifer Weeks, Gregory Munday, Norman Julius Steinert, Hemant Khatri, Matthew Palmer, Laila Gohar, and Rachel Perks

 

Projections of future sea-level rise are critical for informing adaptation planning and risk assessments. However, physical modelling frameworks, due to significant computational requirements, lack the flexibility required for rapid analysis and exploration of the latest global emission scenarios. Data-driven and statistical sea-level emulators can fill this requirement and continue to calibrate themselves to the latest large physical modelling experiments, such as ISMIP, and literature evidence which is published in slower-time - while providing new insights derived from observational constraints and combinations of multiple lines of evidence. Here, we present multi-century sea-level projections using an enhanced version of the ProFSea sea-level emulator tool, and quantify human exposure under high and low-likelihood ice-sheet processes. Due to the flexibility, performance and probabilistic structure of the model, we can explore a large suite of scenarios as well as their observationally constrained counterparts, identify dominant sources of model and process uncertainty, and go further in our analysis to determine human-relevant impacts for vulnerable regions around the world. In addition, we push the emulator out-of-sample to explore its behaviour under idealised very-high emission and overshoot scenarios - a potentially critical limitation of non-physically based emulators.

How to cite: Weeks, J., Munday, G., Steinert, N. J., Khatri, H., Palmer, M., Gohar, L., and Perks, R.: Multi-century sea-level projections and human impacts under the indicative ScenarioMIP-CMIP7 forcings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18937, https://doi.org/10.5194/egusphere-egu26-18937, 2026.

EGU26-19879 | ECS | Orals | CL4.13

Changes in sea-level, regional climate, and future coastlines due to the progressive disintegration of the Greenland and West Antarctic ice sheets 

Christine Kaufhold, Matteo Willeit, Torsten Albrecht, Volker Klemann, and Andrey Ganopolski

Current estimates of sea-level rise suggest nearly half a billion people could live on land vulnerable to temporary flooding by the end of this century, with potentially larger global populations, in addition to ecological and climatological threats, becoming more at risk in the far future when sea-level rise becomes increasingly dominated by melt from the Greenland (GrIS) and Antarctic (AIS) ice sheets. Long-term projections remain uncertain due to differences in models, process understanding and their parameterization with many simulations limited to only to 2100 or 2500 CE. Few studies have examined the multi-millennial response; those that do typically consider the GrIS or AIS alone and the focus is limited to global mean sea-level change, whereas spatial variations in sea-level and its implications for regional climate change are neglected.

Using the fast Earth system model CLIMBER-X, we perform idealized 50 kyr long simulations under pre-industrial CO2 concentrations, in which the GrIS, West Antarctic (WAIS), and combined GrIS+WAIS are progressively disintegrated following a realistic pattern of melt derived from previous studies. We repeat these disintegration experiments for different prescribed constant atmospheric CO2 concentrations, and target at changes in global mean near-surface temperature (ΔGMST) of 0–3 °C. Simulations start from a non-equilibrium state based on a dedicated transient simulation of the last glacial cycle with prescribed greenhouse gases and ice-load history, resulting in a present-day disequilibrium in bedrock elevation. These idealized experiments are able to quantify global and regional climate and sea-level response across varying levels of ice sheet melt and GMST change, as well as ocean thermal expansion.

First, we assess the individual impact of a GrIS+WAIS disintegration. Progressively disintegrated ice sheets leads to further warming on top of the targeted ΔGMST due to the albedo effect. However, we find that the added-up response from the individual ice sheet experiments do not reproduce the results from the GrIS+WAIS experiment, indicating the presence of nonlinear feedbacks when combined. There are significant interhemispheric differences, with regional temperatures in the added-up response from the individual ice sheet experiments differing by -13–3 °C when compared to the GrIS+WAIS experiment under pre-industrial CO2 concentrations. These numbers tend to grow as ΔGMST increases.

Second, we compare our experiments to those initialized from a pre-industrial equilibrium to assess the effect of bedrock uplift, differing spatial variations in sea-level, and coastline migration. Whereas bedrock uplift has little effect on ΔGMST, it partially compensates long-term inundation in areas like Northern Europe and Hudson Bay. Hazard maps of progressive inundation are shown for the different simulations, illustrating plausible future coastlines. A dedicated experiment with the complete disintegration of the GrIS+AIS (all ~65m) is also shown. The presented results highlight the sensitivity of regional climate and sea-level to ongoing cryospheric change, and provide a framework to assess the long-term effect of ice sheet melt in the Earth system.

How to cite: Kaufhold, C., Willeit, M., Albrecht, T., Klemann, V., and Ganopolski, A.: Changes in sea-level, regional climate, and future coastlines due to the progressive disintegration of the Greenland and West Antarctic ice sheets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19879, https://doi.org/10.5194/egusphere-egu26-19879, 2026.

EGU26-20445 | Orals | CL4.13 | Highlight

On the predictability of Antarctica's contribution to sea level rise 

Cyrille Mosbeux, Gael Durand, Nicolas Jourdain, Fabien Gillet-Chaulet, Justine Caillet, Gerhard Krinner, Robert Nicholls, Charles Amory, Frederik Boberg, Suzanne Bevan, Tijn Berends, Stephen Cornford, Violaine Coulon, Tamsin Edwards, Goelzer Heiko, Christoph Kittel, Ann Kristin Klose, Gunter Leguy, William Lipscomb, and Ruth Mottram and the PROTECT

Antarctica’s contribution to global sea-level rise is accelerating, yet projections from ice-sheet models continue to span a wide range despite sustained advances in resolution and physical realism. Using a coordinated ensemble of simulations from the H2020 European PROTECT project, we assess both the ability of six state-of-the-art ice-sheet models to reproduce observed Antarctic mass loss since the early 1990s and the extent to which present-day behaviour constrains future evolution.

Across most of the ice sheet, model agreement with observations is limited, reflecting strong sensitivity to model structure and internal dynamics rather than to external forcing alone. In sharp contrast, the Amundsen Sea sector of West Antarctica exhibits a persistent and robust relationship between modelled present-day mass-loss rates and projected sea-level contribution that extends to the end of the twenty-first century and beyond. This sector emerges as the only region where contemporary observations retain demonstrable predictive power for long-term outcomes, while elsewhere compensating processes dominate. Our results identify a fundamentally regional limit of predictability for the Antarctic Ice Sheet, highlighting where emergent constraints can meaningfully inform projections—and where uncertainty is likely irreducible with current models and observations.

How to cite: Mosbeux, C., Durand, G., Jourdain, N., Gillet-Chaulet, F., Caillet, J., Krinner, G., Nicholls, R., Amory, C., Boberg, F., Bevan, S., Berends, T., Cornford, S., Coulon, V., Edwards, T., Heiko, G., Kittel, C., Klose, A. K., Leguy, G., Lipscomb, W., and Mottram, R. and the PROTECT: On the predictability of Antarctica's contribution to sea level rise, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20445, https://doi.org/10.5194/egusphere-egu26-20445, 2026.

EGU26-20690 | Orals | CL4.13

Sea-level rise scenarios and information to support effective risk assessment and adaptation planning 

Robert Nicholls, Jason Lowe, Jochen Hinkel, and Susan Hanson

Sea-level rise (SLR) information and scenarios have improved greatly over the last few decades. This includes spatially explicit online tools which facilitate access for coastal risk and adaptation users. There is also a greater need to provide guidance on the use of this information including the median and extreme projections. In addition to SLR science aspects this also requires consideration of the user perspective and the diverse decisions that are using SLR information. Some would argue that the user perspective and needs are the starting point for such analysis. Key user issues include risk tolerance and timescale of the decision. Co-production of appropriate SLR information among practitioners, policymakers and SLR scientists will support well-informed choices concerning the appropriate SLR information and its application in coastal adaptation and practise. This is a key step in mainstreaming SLR adaptation to a routine, operational activity which is a priority as SLR accelerates. SLR projections around the median are increasingly well understood and consistent across sources, with growing confidence in the methods used to develop them. However, less likely high-end SLR responses remain uncertain, mainly reflecting knowledge gaps and quantitative uncertainties in the Greenland/Antarctic ice sheet components of SLR. Consideration of this information, where appropriate, is important to understand the range of risks and avoid maladaptation. Despite this uncertainty, many decisions on maintenance, upgrade and new adaptation actions need to be made today or in the near future before we expect this uncertainty to be significantly addressed. There is a danger of both under- and over-preparing for these tail risks. Different approaches to tackling decisions under uncertainty will be considered. Taking an adaptive (or multi-step)  approach has many benefits implying a learning approach to adaptation and the need to assess the evolution of SLR over time in addition to projections. The implications for sea-level and associated ice sheet science will be considered.

How to cite: Nicholls, R., Lowe, J., Hinkel, J., and Hanson, S.: Sea-level rise scenarios and information to support effective risk assessment and adaptation planning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20690, https://doi.org/10.5194/egusphere-egu26-20690, 2026.

EGU26-21975 | Posters on site | CL4.13

High-Resolution Modeling Confirms a La Niña-like Forced Sea Level Response in CESM 

John Fasullo and Steve Nerem

Patterns of sea level rise (SLR) and surface warming are tightly coupled, though strong S/N in SLR makes it ideal for identifying forced responses. While climate model ensembles provide an estimate of the forced SLR pattern, standard-resolution models poorly resolve key components of the coupled climate response, including ocean eddies and atmospheric and oceanic fronts. The importance of these small-scale features to regional SLR trends constitutes a major uncertainty in current simulations. Here, the improvements provided through high-resolution (HR) modeling are demonstrated using the recently released MESACLIP experiment, a 10-member ensemble spanning 1920-2100 that is unique for its HR atmospheric (0.25º) and oceanic (0.1º) components. Through comparison with standard-resolution simulations, including a nominal 1º version of the model used in MESACLIP, a fundamental alteration in both the pattern and magnitude of forced regional SLR in the MESACLIP simulations is demonstrated. Agreement between 30-year simulated trends and satellite altimetry is greatly improved and altimeter-era emergence of a La Niña-like forced response is identified in the Pacific and Southern Oceans. These findings suggest that forcing contributes significantly to the ongoing La Niña-like changes in the Pacific ocean and that significant improvements in forced climate change patterns, including those in regional SLR, can be realized through HR climate model ensembles.

How to cite: Fasullo, J. and Nerem, S.: High-Resolution Modeling Confirms a La Niña-like Forced Sea Level Response in CESM, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21975, https://doi.org/10.5194/egusphere-egu26-21975, 2026.

The rapid human-driven depletion of groundwater resources across the Indian subcontinent poses a critical threat to long-term water and food security. The Northwestern Indo-Gangetic Alluvial Plain (NIGAP) is experiencing persistent groundwater depletion due to the combined effects of intensive agricultural and industrial demands. This region, situated on the seismically active Himalayan Foreland Basin, relies heavily on its vast Quaternary alluvial aquifer system. In this study, we integrate multiple geodetic approaches to quantify the secular mass loss in this water-stressed region and partition it into changes in total water and groundwater storage (TWS and GWS).

We analyze time series of TWS changes observed at 300-400 km spatial resolution by the Gravity Recovery and Climate Experiment (GRACE/GRACE-FO) missions from 2002 to 2024. These basin-scale mass estimates are compared with hydrological mass change signals inferred from high-resolution vertical land motion (VLM) derived from Interferometric Synthetic Aperture Radar (InSAR), complemented by continuous Global Positioning System (GPS) measurements. The vertical deformation field derived from InSAR and GPS data across NIGAP reveals aquifer compaction driven by pore pressure decline, enabling the quantification of GWS loss through poroelastic compaction models. However, regions outside the aquifer system exhibit elastic uplift of the Earth’s crust in response to reductions in TWS at and beneath the surface. To convert this elastic response into an equivalent TWS change, we implement an inverse elastic half-space model that incorporates observed surface deformation, along with the known elastic and hydrogeological properties of the study area.

Keywords: Groundwater Depletion, Geodetic Measurements, Elastic Half-Space, Indo-Gangetic Plain.

How to cite: More, S., Werth, S., Tiwari, V., and Tiwari, A.: Quantifying Groundwater Storage Loss in The Northwestern Indo-Gangetic Alluvial Plain Using Integrated Geodetic Measurements and Geophysical Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1643, https://doi.org/10.5194/egusphere-egu26-1643, 2026.

EGU26-5221 | ECS | Posters on site | G3.4

First Results for Simulation Environment using Multi-Sensor Network Observing Hintereisferner  

Katharina Lechner, Martin Rückamp, and Roland Pail

Glaciers are vulnerable to the impacts of climate change, making them a dynamic and rapidly transforming element of the Earth system. The consequences of these changes extend far beyond the polar and mountain regions, affecting ecosystems and water resources globally. Challenges such as flood risks and hazards like rock moraines underscore the importance of understanding this part of the ecosystem. Monitoring and measuring glacial environments are essential not only for mitigating risks but also for advancing scientific knowledge. By studying the dynamics of glaciers, scientists can gain a deeper understanding of their interactions with the Earth's climate system and better predict future changes.

The alpine glaciers have been research areas of several institutes for different geodetic sensors for over 150 years. The current challenge lies in leveraging observational data to develop a glacier model that can assimilate geodetic observations. This research aims to design an optimized geodetic sensor network that enhances the integration of field observations into glacier modeling. Both simulations and real-data processing should be considered. Sensitivity studies evaluate first the data products themselves and second the model’s response to various data inputs, identify observation errors, and refine the network design.

At this stage, a framework for a closed-loop simulation environment tailored to the Hintereisferner is presented. This environment should enable systematic assessment of sensor performance, network accuracy, and future scalability on a simulation basis. Spatial and temporal resolution of the ground truth and the observation methods are discussed. Different sensors are introduced in terms of spatial resolution and measurement accuracy. Initial results from sensitivity studies using different sensors are presented. Additionally, challenges in implementing the simulation environment are discussed.

How to cite: Lechner, K., Rückamp, M., and Pail, R.: First Results for Simulation Environment using Multi-Sensor Network Observing Hintereisferner , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5221, https://doi.org/10.5194/egusphere-egu26-5221, 2026.

EGU26-5720 | ECS | Orals | G3.4

Assessing the Potential of Next-Generation Gravity Missions for Estimating Total Drainable Water Storage 

Alireza Sobouti, Mohammad J. Tourian, Peyman Saemian, Cuiyu Xiao, Benjamin Kitambo, and Nico Sneeuw

Total Drainable Water Storage (TDWS) represents the fraction of terrestrial water storage that can drain naturally from a basin. It is a key indicator of basin-scale hydrological responses, acting as a proxy for a basin’s water-retention capacity  and  availability for ecosystems and society. Satellite gravimetry provides a unique observational constraint on terrestrial water storage changes by sensing gravity variations caused by the redistribution of water mass on and beneath the land surface. While current missions such as GRACE and GRACE-FO successfully observe total water storage anomalies, they do not measure absolute water storage or any proxy of it. TDWS must therefore be inferred by interpreting gravity-based storage changes through the storage–runoff relationship, which governs how storage variations translate into drainage and river discharge. However, the limited effective spatial resolution of current gravity missions restricts robust analyses to large river basins and prevents investigations of smaller basins and sub-basin-scale hydrological processes. These limitations lead to the question of what improvements in TDWS estimation can be expected from next-generation gravity missions with enhanced spatial resolution and sampling.

In this study, we assess the potential impact of next-generation gravity missions, specifically NGGM and MAGIC, on the global-scale estimation of TDWS. We use simulated gravity observations, with two generations of the ESA Earth System Model (ESM2.0 and ESM3.0) providing the Total Water Storage Anomaly (TWSA) as the reference signal. TDWS is then estimated using a storage–runoff relationship, with TWSA representing storage and runoff taken from in situ observations. All mission scenarios, including GRACE-C, NGGM, and MAGIC, are processed using an identical TDWS estimation framework, ensuring that differences in the resulting TDWS parameters arise solely from mission design characteristics such as spatial resolution, temporal sampling, and noise levels.

Mission performance is evaluated at the basin scale by comparing basin-averaged total water storage anomalies and TDWS-related parameters against ESM reference values. The impact of each mission is quantified in terms of (i) accuracy, defined as the closeness of mission-based parameters to the model reference, and (ii) parameter uncertainty, assessed through confidence intervals derived from the storage–runoff fitting. The analysis is further stratified by basin size, storage–discharge coupling, and hydrological complexity.

The results show that NGGM and MAGIC reproduce basin-scale TDWS parameters more accurately than a GRACE-C–like scenario, particularly for smaller basins. Comparison with the ESM reference demonstrates that future missions reduce parameter errors, tighten confidence intervals, and better capture differences in hydrological behavior across basins. At the same time, the study demonstrates that improved gravity observations must be complemented by physically meaningful storage–runoff relationships to fully exploit the potential of future missions. A comparison between results obtained from ESM2.0 and ESM3.0 is therefore required to assess how advances in the representation of basin-scale hydrological processes affect the evaluation of future mission impacts on complex hydrological behavior.

This work was carried out within the SING project, funded by the European Space Agency under the ‘NGGM and MAGIC Science and Applications Impact Study’ ESA Contract No. 4000145265/24/NL/SC.

How to cite: Sobouti, A., Tourian, M. J., Saemian, P., Xiao, C., Kitambo, B., and Sneeuw, N.: Assessing the Potential of Next-Generation Gravity Missions for Estimating Total Drainable Water Storage, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5720, https://doi.org/10.5194/egusphere-egu26-5720, 2026.

Changes in terrestrial water storage (TWS) induce measurable elastic deformation of the Earth’s surface, known as hydrological loading. GNSS observations quantify these surface deformations and, despite being point measurements, they contain the full spectrum of the hydrological loading. Likewise, GRACE and GRACE-FO satellite missions support the monitoring of these hydrological loads, but their coarse spatial resolution (i.e., long-wavelength components) limits the characterization of short-wavelength and localized hydrological processes. Given these two different yet complementary geodetic remote sensing technologies, recent efforts have been made to combine them for recovering high-resolution TWS fields.

Building on these recent efforts, we adopted a remove-restore framework, a widely used technique in regional gravity field modeling, to invert TWS variations from GNSS-derived vertical displacements. In this framework, GRACE-based hydrological loading is first synthesized into vertical deformation up to degree and order 60, and then removed from GNSS observations, isolating residual displacements dominated by sub-GRACE-scale hydrological signals (i.e., short-wavelength components). These residuals are then inverted using a modified elastic Green’s functions to recover residual high-resolution TWS anomalies, which are subsequently restored with the long-wavelength GRACE signal to obtain high-resolution TWS anomaly fields. We applied the method to Chile, a region characterized by strong hydro-climatic gradients and significant tectonic activity, which served as a challenging testbed for the inversion of hydrological loading into high-resolution TWS.

Our results showed that the remove–restore approach enhances both the spatial detail and amplitude of TWS variations compared to GRACE alone, while preserving consistency with large-scale mass changes. Comparisons with land surface and hydrological model outputs indicated improved representation of regional and local hydrological variability. Overall, this exercise demonstrates the potential of integrating GNSS and GRACE/GRACE-FO through a remove-restore strategy to reconcile complementary geodetic observations and better resolve multi-scale water storage dynamics.

 
 

 

 

How to cite: Ferreira, V., Zeng, Z. B., and Montecino, H.: High-resolution terrestrial water storage from GNSS vertical deformation using a remove–restore hydrological loading framework: Application to Chile, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6155, https://doi.org/10.5194/egusphere-egu26-6155, 2026.

EGU26-6604 | Orals | G3.4

A dataset of long daily TWS changes over Europe, inferred from vertical displacements measured by GPS 

Anna Klos, Artur Lenczuk, and Janusz Bogusz

Vertical displacements of Earth’s crust recorded by a set of permanent stations of Global Positioning System (GPS) antennas are used to infer the gridded changes in Terrestrial Water Storage (TWS) using elastic loading theory. Spatial resolution of the resulting gridded TWS changes is dependent on the number of displacement observations available for the region. For several regions around the world, including Europe, dense networks of GPS stations may guarantee high spatial resolution of the inferred gridded TWS changes, far exceeding the spatial resolution of gridded TWS changes that can be obtained from the Gravity Recovery and Climate Experiment (GRACE) observations. Similarly, the daily temporal resolution of gridded TWS changes that we can infer using daily GPS displacements is extremely competitive with monthly GRACE solutions. Both improvements allow for the analysis of regional sub-monthly TWS changes. In this presentation, we showcase a dataset of daily gridded TWS changes over Europe, inferred from vertical displacements measured by more than 4,000 GPS stations across Europe, for a period of 1994-2023. We use the vertical displacements provided by the Nevada Geodetic Laboratory (NGL) and analyze them thoroughly to eliminate the displacements showing apparent changes unrelated to hydrology. We then divide the displacements into three temporal scales of short-term, seasonal and long-term changes to enhance a better understanding of the resulting gridded TWS changes and classify this set of GPS stations into hydrological benchmarks. We then use this benchmark dataset and invert the displacement time series into gridded TWS changes over Europe. We perform several comparisons on regional and local spatial scales with GRACE, hydrological models, and other datasets, and prove that the resulting TWS changes may enhance future analyses of regional hydrological changes.

How to cite: Klos, A., Lenczuk, A., and Bogusz, J.: A dataset of long daily TWS changes over Europe, inferred from vertical displacements measured by GPS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6604, https://doi.org/10.5194/egusphere-egu26-6604, 2026.

EGU26-8530 | ECS | Posters on site | G3.4

Analysis of Three-Dimensional Seasonal deformation induced by GPS and loading models in Yunnan, China 

Yujiao Niu, Guangli Su, Layue Li, Wei Zhan, Min Li, and Yanqiang Wu

Seasonal deformation related to mass redistribution on the Earth’s surface can be recorded by continuous global positioning system (GPS) and simulated by surface loading models. In this study, we compared the three-dimensional seasonal deformation from 27 continuous GPS stations and surface loading models in Yunan, China. A good consistency of vertical seasonal variations can be observed between GPS and loading models, while obvious discrepancies exist in the horizontal seasonal deformation between them, especially for the East component. The reduction ratios of the median amplitudes of GPS annual variations obtained with loading corrections are 39.37%,-18.01% and 56.39% for the North, East and Up components respectively. We found that the significant difference in horizontal annual deformation between GPS and loading models is primarily attributed to the discrepancies of GPS annual phases at different stations. Seasonal vectors are employed to discriminate loading at different spatial scales. The results suggests that the large-scale load is concentrated in the southwest of Yunnan, the disordered horizontal annual phase may be related to local-scale mass loading. In addition, after removing the loading deformation from GPS time series, GPS vertical velocity uncertainties are significantly reduced, with the mean reduction ratio about 9%.

How to cite: Niu, Y., Su, G., Li, L., Zhan, W., Li, M., and Wu, Y.: Analysis of Three-Dimensional Seasonal deformation induced by GPS and loading models in Yunnan, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8530, https://doi.org/10.5194/egusphere-egu26-8530, 2026.

EGU26-9175 | Orals | G3.4

Uplift and subsidence by heavy rains: Hydrogeodesy of Mt. Fuji, Japan 

Kosuke Heki, Shuo Zheng, Jianli Chen, Zizhan Zhang, and Haoming Yan

Active volcanoes often deform by magmatic activities at depth. Here we report that they deform also by hydrological activities induced by rains. By analyzing the daily coordinates of global navigation satellite system stations deployed around the Fuji volcano, the highest mountain of the country in central Japan, we detected transient surface uplift of 1-2 centimeters correlated with heavy rains. We consider they were caused by the expansion of shallow aquifers within Shin-Fuji lava layers. Such hydrological inflation of the volcano, lasting for a day or two, occurs within ~25 km from the summit. The uplift gradually decays with distance and is replaced with large-area subsidence by rainwater loading beyond the end of these lava layers. Subsidence is proportional to daily rains, rather than cumulative rains, suggesting dynamic equilibrium of precipitation and run-off. Understanding such ‘cold’ deformation of active volcanoes would help us correctly interpret ‘hot’ ones by magmatic activities.

How to cite: Heki, K., Zheng, S., Chen, J., Zhang, Z., and Yan, H.: Uplift and subsidence by heavy rains: Hydrogeodesy of Mt. Fuji, Japan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9175, https://doi.org/10.5194/egusphere-egu26-9175, 2026.

EGU26-11420 | Posters on site | G3.4

Comparison of GNSS residuals displacementswith environmental loading models 

Jean-Paul Boy, Paul Rebischung, and Zuheir Altamimi

All geodetic technique observations (DORIS, GNSS, SLR and VLBI) have been processed up to the end of 2024 in order to compute the  second update of the International Terrestrial Reference Frame 2020, namely ITRF2020-u2024 (https://itrf.ign.fr/en/solutions/ITRF2020-u2024). Following the IERS conventions, no environmental loading corrections have been applied besides ocean tides.

We also compute daily GNSS solution using the GINS software in iPPP (precise point positioning with integer ambiguity resolution) for the 2000-2025 period, and orbit/clock products from the CNES/CLS analysis center.

In parallel, the IERS Global Geophysical Fluid Center has provided atmospheric, induced oceanic and hydrological loading estimates for all permanent stations based on the latest ECWMF reanalysis (ERA5) and the barotropic ocean model TUGO-m (http://loading.u-strasbg.fr/ITRF2020/).

In this paper, we present a comparison of both the combined ITRF2020-u2024 and our daily GNSS residual displacements to environmental (atmosphere, ocean and continental hydrology) loading estimates. In more details, we show that the ERA5-based reanalyzes are in better agreement with the geodetic observations than the MERRA2 (Modern-Era Retrospective Analysis for Research and Applications, Version 2) reanalysis. We also show the improvement of the ERA5-land, a re-run of the land component of the ECMWF ERA5 climate reanalysis, versus the original ERA5 hydrological component.

Finally, we also show that a dynamic ocean response to pressure and wind is more suitable to model high frequency ocean non-tidal loading effects than the classical inverted barometer (IB) approximation.

How to cite: Boy, J.-P., Rebischung, P., and Altamimi, Z.: Comparison of GNSS residuals displacementswith environmental loading models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11420, https://doi.org/10.5194/egusphere-egu26-11420, 2026.

EGU26-14041 | Posters on site | G3.4

Terrestrial Quantum Gravimetry for Climate Monitoring: First Measurements in Greenland 

Tim Enzlberger Jensen, Przemyslaw Dykowski, and Adam Ciesielski

During summer 2025, an Absolute Quantum Gravimeter (AQG, manufactured by Exail) was deployed for one week in western Greenland to explore the potential of quantum gravimetry for geodetic observations in an Arctic environment - under remote and harsh field conditions - and to evaluate the sensitivity of absolute gravity measurements to mass redistribution processes associated with glacier dynamics and solid Earth deformation.

For most of the week, the AQG collected measurements at an established gravity point in the hangar of Ilulissat airport (ILUL). For one day, the instrument was transferred by helicopter to another established gravity point in the bedrock near the Greenland Ice Sheet, approximately 50 km inland along the Ilulissat ice stream. The point is co-located with the Kangia North (KAGA) permanent GNSS station, enabling a direct link between absolute gravity, surface deformation and cryospheric mass change signals. The station is located in proximity of the calving front of the Ilulissat glacier, one of the fastest-flowing and most dynamically active glaciers in Greenland.

In this contribution, we present preliminary results from the 2025 campaign and compare them with previous absolute gravity measurements obtained using an absolute A10 gravimeter at both sites. These time-separated absolute gravity observations provide a basis for assessing the potential of AQGs to monitor gravity variations associated with ice and water mass changes together with Glacial Isostatic Adjustment (GIA). We discuss the significance of the observed values, compare them with predicted gravity trends, and assess the credibility and uncertainty of the results under Arctic field conditions. The AQG observations are evaluated as a complement to GNSS and classical absolute gravimetry as a geodetic method for long-term cryospheric monitoring, with the 2025 campaign serving as a baseline for future repeated measurements. The expedition serves as a pilot study for repeated quantum gravimetry observations in Greenland, planned to be continued with a similar instrument in summer 2028.

The campaign was carried out within the project EQUIP-G (funded by the European Commission under the Horizon Europe program, grant number 101215427) and with support from the Danish Climate Data Agency.

How to cite: Jensen, T. E., Dykowski, P., and Ciesielski, A.: Terrestrial Quantum Gravimetry for Climate Monitoring: First Measurements in Greenland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14041, https://doi.org/10.5194/egusphere-egu26-14041, 2026.

EGU26-16776 | Orals | G3.4

Mass Loss of the Antarctic Peninsula ice sheet and its peripheral glaciers from 2007 to 2021 

Maud Bernat, Etienne Berthier, Amaury Dehecq, Romain Hugonnet, Joaquin MC Belart, Naomi Ochwat, Ted Scambos, Peter Kuipers Munneke, Elizabeth Case, Louis-Marie Gauer, and David Youssefi

The Antarctic Peninsula (AP), encompassing the ice sheet and its peripheral glaciers, is a highly dynamic component of the cryosphere, disproportionately contributing to sea level rise. However, a large spread remains between the mass changes estimated using gravimetry, altimetry and the input/output method. Among these techniques, the satellite (radar or laser) altimetry method has a resolution of, at best, 1 km, which is too coarse to resolve the complex pattern of changes in the Peninsula. Therefore, we use digital elevation models (DEMs; 30x30 m) to map elevation changes for the entire Peninsula, combining 476 DEMs derived from SPOT5-HRS satellite images (2006-2008) and 2525 strips of the Reference Elevation Model of Antarctica (2020-2022) to provide a comprehensive 14-year record. We bias-corrected each DEM using near-synchronous ICESat/-2 laser altimetry measurements.

Our observations cover 70% of the AP ice sheet and 60% of its peripheral glaciers, including for regions of the Peninsula poorly studied to date and decipher a spatially complex pattern of elevation changes. After correction with different models of firn air content and solid-earth response, we find that between 2007 and 2021, the AP ice sheet lost -27 ± 9 Gt/yr while its peripheral glaciers lost -14 ± 2 Gt/yr. For the AP ice sheet, our new estimate is 4 to 5 times more negative than the one obtained in IMBIE using purely altimetry data (-6 ± 6  Gt/yr from 2006 to 2018) and in better agreement with gravimetry and the input/output method. Our study highlights the importance of resolving fine scale elevation changes of glaciers and ice sheets. 

How to cite: Bernat, M., Berthier, E., Dehecq, A., Hugonnet, R., Belart, J. M., Ochwat, N., Scambos, T., Kuipers Munneke, P., Case, E., Gauer, L.-M., and Youssefi, D.: Mass Loss of the Antarctic Peninsula ice sheet and its peripheral glaciers from 2007 to 2021, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16776, https://doi.org/10.5194/egusphere-egu26-16776, 2026.

GFZ provides elastic surface deformation estimates caused by atmospheric surface pressure, ocean bottom pressure, terrestrial water storage, and barystatic sea level variations on global grids. To keep those loading deformations consistent with the latest GRACE de-aliasing products AOD1B R07 we updated the loading products by using ECMWF ERA5 atmospheric forcing, the latest MPIOM ocean model, and the latest hydrological model release from LISFLOOD. We present some statistics on the new ESMGFZ loading deformation products to demonstrate its enhanced long-term stability and suitability for the realization of future high accurate terrestrial reference systems. Especially the hydrological loading component benefits now from the new LISFLOOD terrestrial water storage estimates forced with ECMWF ERA5 atmospheric data and simulated on a global high spatial resolution grid of 0.05° to resolve high deformation amplitudes in the vicinity of large rivers, lakes, and dams. The new ESMGFZ loading products cover the period 1960 to the present.

How to cite: Dill, R., Dobslaw, H., and Jensen, L.: New ESMGFZ loading products for global long-term stable elastic surface deformations consistent with ECMWF ERA5 and GRACE de-aliasing AOD1B 07, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17254, https://doi.org/10.5194/egusphere-egu26-17254, 2026.

EGU26-17316 | ECS | Orals | G3.4

Crustal uplift in the Kerguelen Islands from Sentinel-1 InSAR : A consequence of recent ice melting? 

Charlotte Spriet, Kristel Chanard, Raphaël Grandin, Étienne Berthier, Kevin Gobron, Louis-Marie Gauer, and Luce Fleitout

The Kerguelen Islands (49°S, 69°E), a volcanic archipelago in the southern Indian Ocean, have experienced substantial environmental change over recent decades, including significant retreat of the Cook ice cap. The rapid ice loss is expected to induce measurable crustal deformation.

In this study, we use the complete archive of Sentinel-1 SAR imagery acquired since 2015 to examine the present-day deformation field of the Kerguelen Islands. Our small-baseline InSAR time-series analysis reveals a broad ~ 100 km-wide pattern of crustal uplift centered on the Cook ice cap, reaching up to ~ 6 mm/yr. 

To investigate the physical processes driving this uplift, we combine observed change in ice elevation inferred from multiple Digital Elevation Model over the 2015-2025 period with local estimates of shallow elastic properties derived from seismic experiments. Using a layered Cartesian elastic Earth model, we predict the surface deformation resulting from present-day unloading of the Cook ice cap, and compare model predictions to the InSAR-derived deformation field.

We then explore time-dependent deformation scenarios by considering viscoelastic deformation of the solid Earth induced by a range of plausible ice-loss histories over recent decades, and show that recent ice melting in the Kerguelen island can be used to place constraints on the rheology of the Earth’s upper mantle at decadal timescales. Finally, given the volcanic setting of the Kerguelen Islands, we also investigate whether magmatic sources could contribute to the observed long-wavelength uplift pattern.

Overall, this work highlights the potential of InSAR observations in remote subpolar environments to quantify ice-driven deformation and to infer solid Earth rheological properties on decadal timescales.

How to cite: Spriet, C., Chanard, K., Grandin, R., Berthier, É., Gobron, K., Gauer, L.-M., and Fleitout, L.: Crustal uplift in the Kerguelen Islands from Sentinel-1 InSAR : A consequence of recent ice melting?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17316, https://doi.org/10.5194/egusphere-egu26-17316, 2026.

EGU26-18216 | Orals | G3.4

Enhanced mass balance of Antarctica from RINGS airborne grounding line survey 

Rene Forsberg, Carl Leuschen, Andreas Stokholm, Jilu Li, Tim Jensen, Emily Arnold, and Fernando Rodriguez-Morales

Determining the mass balance of Antarctica by satellite gravimetry, altimetry and input-output methods is still suffering from large discrepancies between methods, especially for East Antarctica. Error sources for the different estimation methods include GIA for GRACE/GRACE-FO, firm compaction for satellite altimetry, and poorly known interior snow fall and grounding line mass flux for outlet glaciers in the input-output method. To narrow down uncertainties for the latter, an international SCAR project “RINGS” was initiated in 2023, aiming as a primary goal to cover all major unmapped outlet glaciers with new radar ice thickness data in the coming years. A unique multi-disciplinary airborne remote sensing RINGS campaign was carried out as part of a first circumnavigation of Antarctica 2024/25, using a Twin-Otter as dedicated science aircraft. The airborne campaign instruments included a 30 GHz deep ice sounding radar, a 5 GHz broadband snow radar, along with scanning lidar, nadir and side-looking imagery, and gravimetry, as well as atmosphere monitoring sensors for chemistry and aerosols. In the presentation we outline the results of the RINGS airborne campaign, the impact on the input-output method of the new outlet glacier thicknesses, and compare the changes to current GRACE/GRACE-FO mass balance results.

How to cite: Forsberg, R., Leuschen, C., Stokholm, A., Li, J., Jensen, T., Arnold, E., and Rodriguez-Morales, F.: Enhanced mass balance of Antarctica from RINGS airborne grounding line survey, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18216, https://doi.org/10.5194/egusphere-egu26-18216, 2026.

EGU26-20281 | ECS | Orals | G3.4

The Caspian Sea defines the recent global inland surface water storage decline 

Benjamin M. Kitambo, Mohammad J. Tourian, Peyman Saemian, Omid Elmi, Sly Wongchuig, Daniel Moreira, Maurício C.R Cordeiro, Ayan Santos Fleischmann, Raphael M. Tshimanga, Frederic Frappart, Catherine Prigent, and Fabrice Papa

The quantification of inland surface water storage anomaly (SWSA) and its spatial-temporal variability across rivers, streams, lakes, reservoirs, floodplains, and wetlands is crucial for understanding the role of continental water in the global hydrological and biochemical cycles. Such knowledge is also essential for sustaining human societies and ecosystems. For more than a decade, significant efforts have been devoted to characterising SWSA in some major river basins and globally for only some types of water bodies. However, global SWSA for all surface water bodies simultaneously has not yet been quantified, and its long-term behavior has not yet been investigated. 

Here, we present the first global estimates of SWSA and investigate its long-term behaviour from 1992 to 2020. This is achieved by benefiting from the integration of multi-mission global satellite products, including satellite-derived Surface Water Height (SWH) from nadir altimeters and Surface Water and Ocean Topography (SWOT). Two methods have been coupled to estimate SWSA over each type of surface water body. The first one, a hypsometric curve method, consists of the combination of surface water extent (from the Global Inundation Extent from Multi-Satellite (GIEMS-2 dataset)) with topographic data from the global Digital Elevation Model (DEM), namely Forest And Buildings removed Copernicus DEM (FABDEM). The second one, based on the lake water level – area storage model, combined the simultaneous lake surface water extent and SWH. Our new SWSA dataset agrees well with other existing regional SWSA estimations.

Our results highlight the relevance of the Caspian Sea system in driving the recent global SWSA decline. At the global scale, results including the Caspian Sea provide a significant negative trend of -14 km3 yr-1. Conversely, the exclusion of the Caspian Sea shows a positive trend at 6 km3 yr-1. 

The newly developed global satellite observation-based SWSA dataset enables novel insights as a new source of information for hydrological and multidisciplinary sciences, including data assimilation, land–ocean exchanges, and water management. Moreover, this global dataset is a benchmark of SWOT-based storage products and their evaluation and validation.

How to cite: M. Kitambo, B., J. Tourian, M., Saemian, P., Elmi, O., Wongchuig, S., Moreira, D., C.R Cordeiro, M., Santos Fleischmann, A., M. Tshimanga, R., Frappart, F., Prigent, C., and Papa, F.: The Caspian Sea defines the recent global inland surface water storage decline, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20281, https://doi.org/10.5194/egusphere-egu26-20281, 2026.

Variations in surface temperature and groundwater pressure within aquifer systems generate internal thermoelastic and poroelastic strain in the shallow subsurface, producing surface deformation and crustal stress perturbations. We develop a general mathematical framework to compute surface displacements and stresses at depth driven by internal strain, accounting for realistic mechanical properties of the Earth, including depth-dependent layering and lateral heterogeneities. 
We show that variations in surface temperature induce deformation below layers affected by internal strain and surface horizontal displacements that scale with the Young’s modulus of the shallow layers where internal strain occurs. Because these layers generally have weak elastic moduli across continental regions (soils, weathered rock, etc.), long-wavelength thermoelastic horizontal deformation is predicted to be negligible. In contrast, vertical displacements driven by thermal expansion within shallow weak layers are expected to reach the millimeter level, implying that thermoelastic effects should be considered when interpreting GNSS signals, in particular at the annual timescale.
At regional scale, lateral contrasts in elastic properties, such as transitions from bedrock to sedimentary basins or across fault damage zones, can produce annual thermoelastic horizontal displacements up to a few mm. The associated annual thermoelastic stress perturbations at depths of a few km may reach several kPa, locally exceeding stresses induced by seasonal hydrological loading, suggesting a potential contribution of surface temperature forcing observed seasonal modulation of seismicity. Over longer timescales, progressive climate-driven warming may also cause non-negligible stress perturbations in intraplate regions. 
Using the same formalism, we investigate deformation and stresses induced by poroelastic pressure variations in aquifer systems. We show that for 10 m variations of the water table, vertical displacements of a few mm to a few cm are expected and lateral variations of elastic properties can generate horizontal deformation of a few mm and crustal stress perturbations of several kPa.

How to cite: Chanard, K. and Fleitout, L.: Thermoelastic and poroelastic deformation of the solid Earth driven surface temperature and groundwater level variations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20492, https://doi.org/10.5194/egusphere-egu26-20492, 2026.

EGU26-20596 | Posters on site | G3.4

Evaluating different-scale hydrological corrections against high-precision terrestrial gravity time series at the Geodetic Observatory Wettzell, Germany 

Anna Winter, Marvin Reich, Patricio Yeste, Ezequiel D. Antokoletz, Andreas Güntner, and Hartmut Wziontek

Hydrological monitoring methods usually observe water storage changes in specific depths or for a limited number of storage compartments and are often representative for a small volume only. In contrast, gravity measurements are sensitive to mass changes as a spatially integrated signal. This makes them a valuable complementary tool for monitoring total water storage changes. The hydrological contribution to the time-variable gravimetric signal often plays a major role for the overall signal dynamics. Nevertheless, there is still a lack of understanding the influence of the local hydrological dynamics at many terrestrial gravity stations. Thus, advancing the hydrological corrections of gravity signals is highly valuable for improving the interpretation of gravity measurements with respect to other processes of interest, e.g., geodynamic, atmospheric or ocean-loading effects. At the same time, high-precision gravity measurements provide a reliable validation to mass-variations as represented by hydrological models.

In this case study, we consider the Geodetic Observatory Wettzell (GOW), located in the river Regen catchment in a low mountain range in East Bavaria, Germany. Here, long-term stable records of superconducting gravimeters (SGs) are available at three different points at the observatory within a distance of about 200 meters. Moreover, an extensive hydrological sensor network has been operated at GOW for more than a decade, which allows for a precise consideration of local effects. Dividing the hydrological effects into local, regional and global contributions, the regional component is calculated based on the mesoscale Hydrologic Model (mHM, Helmholtz Centre for Environmental Research – UFZ), implemented for the river Regen catchment with a spatial resolution of one kilometer and forced with national and global meteorological data sets. Global contributions are considered from various models, including MERRA-2 and several GLDAS solutions.

To assess the efficiency of a small-scale versus a large-scale approach for hydrological corrections, we evaluate all hydrological contributions against gravity residuals, after precise removal of tides, atmospheric, non-tidal ocean loading and polar motion effects. We focus on the consistent combination of each contribution and the impact of local influences, e.g., finely resolved topography in the vicinity of the gravimeters and the effect of buildings. First results show that changing the approach for, or neglecting the local contribution can easily double the total hydrological effect. This emphasizes the importance of carefully considering local effects in the hydrological gravity modelling, in particular at stations with a marked subsurface complexity and heterogeneity like GOW.

How to cite: Winter, A., Reich, M., Yeste, P., Antokoletz, E. D., Güntner, A., and Wziontek, H.: Evaluating different-scale hydrological corrections against high-precision terrestrial gravity time series at the Geodetic Observatory Wettzell, Germany, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20596, https://doi.org/10.5194/egusphere-egu26-20596, 2026.

EGU26-21216 | Posters on site | G3.4

Towards the coupling of a glacier and a hydrological model (OGGM and OS LISFLOOD) for improved loading estimations 

Henryk Dobslaw, Robert Dill, and Laura Jensen

Modelling crustal loading deformations is crucial for various geodetic applications, including the realization of precise and stable terrestrial reference frames. Commonly, hydrological, atmospheric and oceanic models are used to predict surface deformations. But also cryospheric deformations are not negligible considering the accelerating melting of glaciers, and glacier models exist to estimate cryospheric mass variations. However, it is not appropriate to just complement the existing hydrological model with the glacier model estimates as part of the glacier induced deformations are already taken into account by the hydrological model via simplified snow routines, which would lead to double-counting of masses.

A consistent way to consider glacier mass variations in deformation studies would be to couple a hydrological model with a glacier model. While on a basin scale this has been done before, large-scale or even global coupling approaches are still rare partly due to the heterogeneous glacier behavior and relatively small extent of glaciers (often smaller than the grid cell size of the global model). The Open Global Glacier Model (OGGM) is designed for global glacier modelling, and thus, a suitable candidate for a global coupling. Here we present first steps towards coupling OGGM with OS LISFLOOD, an open-source global hydrological model running with a global 0.05° spatial resolution previously used for geodetic applications.

As a first case study, we chose the Fraser river basin in North America. We initially conduct model runs separately with OGGM for selected glaciers contained in the study area, and with OS LISFLOOD to obtain mass storage estimates particularly for the snow compartment. Comparison of both model results gives an impression of the potential double-counting of mass if both models were applied separately, and reveals challenges in a possible coupling workflow. For example, OGGM output is stored per glacier, and thus has to be summed per grid cell in order to pipeline it to grid-based OS LISFLOOD. Furthermore, OS LISFLOOD would have to be adjusted to take input from OGGM in glaciated regions with varying extent.

How to cite: Dobslaw, H., Dill, R., and Jensen, L.: Towards the coupling of a glacier and a hydrological model (OGGM and OS LISFLOOD) for improved loading estimations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21216, https://doi.org/10.5194/egusphere-egu26-21216, 2026.

EGU26-22109 | ECS | Orals | G3.4

Remote Sensing-Based Framework for Detecting and Interpreting Permafrost Terrain Hydrologic Connectivity 

David Richards IV, Trina Merrick, Robert Liang, Andrei Abelev, Michael Vermillion, Maya Maciel-Seidman, and Sofia Grossman

Arctic coasts are among the most vulnerable landscape on Earth, where periglacial terrain undergoes thermal contraction and expansion through seasonal freeze–thaw cycles. Along the Utqiaġvik (formerly Barrow), Alaska coastline, shifting thermal regimes have accelerated ice wedge degradation, influenced by the evolution of polygonal trough networks. However, accurately mapping trough structure, variability, and hydrologic connectivity across spatial scales remains challenging. This study integrates high-resolution remote sensing and terrain modeling to investigate the relationship between surface hydrology and ice wedge polygon morphology. Using a 0.5 m resolution LiDAR-derived digital elevation model (DEM), ice wedge polygons were manually delineated and compared with Thiessen (Voronoi)  polygons to evaluate differences in structure, spatial extent, and representation of natural variability. Intersection analyses revealed significant discrepancies in boundary alignment and area estimates between the two approaches. Hydrologic influences on polygon development were assessed through compound terrain analysis, drainage network extraction, and surface flow modeling. Results show strong spatial correspondence between modeled flow paths and mapped trough networks, indicating that surface hydrology plays a key role in ice wedge thaw and trough evolution. Calculated hydrologic and morphometric parameters suggest high runoff potential, driven by flat terrain, permafrost-limited infiltration, dense drainage networks, and short overland flow paths. High TWI (> 12) and SPI (> 60) values mark zones of concentrated surface saturation and flow accumulation, often coinciding with trough depressions. Despite high runoff potential, minimal gradients lead to slow-moving flow and persistent surface ponding, contributing to widespread wetland formation. This integrated approach demonstrates the value of combining high-resolution topographic data with hydrologic modeling to improve detection and interpretation of permafrost terrain features. The framework developed offers a scalable method for monitoring Arctic terrain dynamics and enhances remote sensing applications for assessing permafrost vulnerability.

How to cite: Richards IV, D., Merrick, T., Liang, R., Abelev, A., Vermillion, M., Maciel-Seidman, M., and Grossman, S.: Remote Sensing-Based Framework for Detecting and Interpreting Permafrost Terrain Hydrologic Connectivity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22109, https://doi.org/10.5194/egusphere-egu26-22109, 2026.

EGU26-2310 | ECS | Posters on site | NP1.2

Reduced Complexity Model Intercomparison Project Phase 3: protocol and preliminary results 

Alejandro Romero-Prieto, Marit Sandstad, Benjamin M. Sanderson, Zebedee R. J. Nicholls, Norman J. Steinert, Thomas Gasser, Camilla Mathison, Jarmo Kikstra, Thomas J. Aubry, Katsumasa Tanaka, Konstantin Weber, and Chris Smith

Reduced-complexity models (RCMs) are a critical tool in climate science. Their computational efficiency enables applications beyond the reach of more complex models, including uncertainty quantification, the integration of multiple lines of evidence via ensemble constraining, and running large scenario sets in the span of a few days. Thanks to these capabilities, RCMs played important roles in previous IPCC assessments, and are poised to play an important role in the upcoming Seventh Assessment Report (AR7). A key example is evaluating the climate response to the thousands of emissions scenarios in the peer-reviewed literature created with integrated assessment models. However, whether/which RCMs are suitable for performing such a task is contingent on their ability to faithfully emulate the behaviour of more complex models and observed climate change.

The Reduced-Complexity Model Intercomparison Project (RCMIP) was established to assess this capability, as well as to better understand inter-RCM differences (Nicholls et al., 2020; Nicholls et al., 2021). Here, we introduce the protocol for the third and latest phase, RCMIP3. This phase focuses on two priorities. First, it provides a common set of observational benchmarks to be optionally used for ensemble constraining prior to submission, with the objective of mitigating discrepancies arising from different calibration methodologies and facilitating a clearer assessment of intrinsic model differences. Second, it requests an expanded set of variables and experiments from modelling teams to enable a more thorough evaluation of the carbon cycle representation in these models – a key gap in previous RCMIP phases. Additionally, RCMIP3 includes many of the experiments in the “Assessment Fast Track" (AFT) of the Coupled Model Intercomparison Project Phase 7 (CMIP7). As a result, RCMIP3 will improve our understanding of future model differences under these experiments, in addition to providing the community with valuable early projections.

The presentation will outline the RCMIP3 protocol and highlight the types of analyses it enables, along with preliminary results. By explicitly comparing RCM outputs with both ESM simulations and observations, RCMIP3 aims to strengthen the linkage across the climate-model hierarchy as well as evaluating and showcasing the suitability of RCMs for climate assessment.

Nicholls, Z., Meinshausen, M., Lewis, J., Corradi, M.R., Dorheim, K., Gasser, T., Gieseke, R., Hope, A.P., Leach, N.J., McBride, L.A., Quilcaille, Y., Rogelj, J., Salawitch, R.J., Samset, B.H., Sandstad, M., Shiklomanov, A., Skeie, R.B., Smith, C.J., Smith, S.J., Su, X., Tsutsui, J., Vega-Westhoff, B. and Woodard, D.L. 2021. Reduced Complexity Model Intercomparison Project Phase 2: Synthesizing Earth System Knowledge for Probabilistic Climate Projections. Earth’s Future. 9(6), https://doi.org/10.1029/2020EF001900.

Nicholls, Z.R.J., Meinshausen, M., Lewis, J., Gieseke, R., Dommenget, D., Dorheim, K., Fan, C.-S., Fuglestvedt, J.S., Gasser, T., Golüke, U., Goodwin, P., Hartin, C., Hope, A.P., Kriegler, E., Leach, N.J., Marchegiani, D., McBride, L.A., Quilcaille, Y., Rogelj, J., Salawitch, R.J., Samset, B.H., Sandstad, M., Shiklomanov, A.N., Skeie, R.B., Smith, C.J., Smith, S., Tanaka, K., Tsutsui, J. and Xie, Z. 2020. Reduced Complexity Model Intercomparison Project Phase 1: introduction and evaluation of global-mean temperature response. Geoscientific Model Development. 13(11), pp.5175–5190, https://doi.org/10.5194/gmd-13-5175-2020.

How to cite: Romero-Prieto, A., Sandstad, M., Sanderson, B. M., Nicholls, Z. R. J., Steinert, N. J., Gasser, T., Mathison, C., Kikstra, J., Aubry, T. J., Tanaka, K., Weber, K., and Smith, C.: Reduced Complexity Model Intercomparison Project Phase 3: protocol and preliminary results, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2310, https://doi.org/10.5194/egusphere-egu26-2310, 2026.

EGU26-4264 | Posters on site | NP1.2

METEOR 1.5 a spatial emulator for fast and relevant responses to impact questions 

Marit Sandstad, Benjamin Sanderson, Norman Steinert, and Shivika Mittal

Here we present an extended version of the forcing-driven and overshoot-aware spatial impacts emulator METEOR, which now includes functionality to emulate monthly outputs which include seasonality and natural variability, with the option to produce large distribution ensembles for a point, regional average or spatial domain.  The philosophy of METEOR entails fast training on few and widely available datasets, sufficiently fast to be run on-the-fly and removing the need to archive large datasets and allowing interactive coupling with integrated assessment frameworks to simulate impacts directly.  METEOR1.5 introduces a state dependent seasonal model and an autoregressive spatial, state-dependent noise model which can produce distributions of realisations conforming to the climatic trends and distributional properties of the emulated model    Integrated impact modules allow the direct emulation of human and ecological stressors which are computed from easily retrained emulated climates to answer regional questions. 

How to cite: Sandstad, M., Sanderson, B., Steinert, N., and Mittal, S.: METEOR 1.5 a spatial emulator for fast and relevant responses to impact questions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4264, https://doi.org/10.5194/egusphere-egu26-4264, 2026.

EGU26-5437 | ECS | Orals | NP1.2

When and where higher-resolution climate data improve impact model performance 

Johanna Malle, Christopher Reyer, and Dirk Karger and the ISIMIP modellers and sector coordinators

Climate impact assessments increasingly rely on high-resolution climate and forcing datasets, under the premise that finer detail enhances both the accuracy and the policy relevance of projections. Systematic evaluations of when and where higher resolution data improve model outcomes remain limited, and it is still unclear whether increasing spatial resolution consistently enhances climate impact model performance across application areas, regions, and forcing variables. Here we show that improvements in climate input accuracy and impact model performance are most pronounced when moving from coarse (60 km) to intermediate (10 km) resolution, while further refinement to 3 km and 1 km provides more modest and inconsistent benefits. Using the cross-sectoral model simulations from the Inter-Sectoral Impact Model Intercomparison Project (ISIMIP), we demonstrate that higher resolution substantially improves model skill in temperature-sensitive impact models and topographically complex regions, whereas precipitation-driven and low-relief systems show less consistency to increase performance with resolution. For temperature, both climate inputs and model outputs improved most strongly at the 60 km → 10 km transition, with diminishing gains at finer scales. A similar result emerged for precipitation, although some models even exhibited reduced performance when resolution increased beyond 10 km. These results highlight that optimal resolution depends on sectoral and regional context, and point to the need for improving model process representation and downscaling techniques so that added spatial detail can translate into meaningful performance gains. For data providers, this implies prioritizing investments in resolutions that maximize improvements where they matter most, while for modeling groups and users, it underscores the need for explicit benchmarking of resolution choices. More broadly, this work advances the design of consistent, efficient, and policy-relevant multi-sectoral climate impact assessments by clarifying when high-resolution data meaningfully enhance outcomes.

How to cite: Malle, J., Reyer, C., and Karger, D. and the ISIMIP modellers and sector coordinators: When and where higher-resolution climate data improve impact model performance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5437, https://doi.org/10.5194/egusphere-egu26-5437, 2026.

EGU26-5816 | ECS | Posters on site | NP1.2

Defining an early warning method for an AMOC collapse based on ensemble statistics 

Dániel Jánosi, Ferenc Tamás Divinszki, Reyk Börner, and Mátyás Herein

The Atlantic Meridional Overturning Circulation (AMOC) is a crucial climate component, as its potential collapse would constitute a significant response to Earth’s changing climate. This critical transition has been the subject of numerous studies over the years, both from the aspect of climate modeling and dynamical systems theory. In the context of the latter, climate change is a process in which a complex, chaotic-like system possesses time-dependent parameters, in the form of e.g. the growing CO2 concentration. It has been known that such systems have a chaotic attractor which is also time-dependent, a so-called snapshot attractor. Such objects, and thus the systems they describe, can only be faithfully represented by a probability distribution over an ensemble of simulations, so-called parallel climate realizations.

Based on this probability distribution, we define a novel early warning indicator for crucial transitions such as an AMOC collapse. The AMOC is said to possess a multistable quasipotential landscape, and the collapse is a transition between stable states. We argue that, from the point of view of statistical physics, this is analogous to a phase transition, but in a non-adiabatic setting. As such, the variance of the distribution over the ensemble is expected to develop a local maximum around the transition point, giving rise to a potential early warning by identifying the preceding maximum of its derivative. This method is first demonstrated on a conceptual climate model, before the analysis is carried out on ensemble simulations from the ACCESS-ESM model. The analysis in the former case is simpler, while in the latter, one has to contend with the dependence of the AMOC strength on spatial coordinates, resulting in multiple early warning points for different depths and latitudes.

How to cite: Jánosi, D., Divinszki, F. T., Börner, R., and Herein, M.: Defining an early warning method for an AMOC collapse based on ensemble statistics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5816, https://doi.org/10.5194/egusphere-egu26-5816, 2026.

Offline aridity and drought indices have often implied widespread terrestrial drying under a warming environment, while Earth system models (ESMs) have projected modest changes in land-surface water fluxes. This persistent divergence has been typically attributed to missing vegetation physiological processes in offline frameworks. However, we here show that a more foundational cause is a structural inconsistency embedded in those diagnostics. Conventional potential evapotranspiration (PET) formulations can violate the assumption that precipitation (P) and atmospheric evaporative demand act as independent climatic constraints in the Budyko framework. Using open-water Penman and vegetation-responsive Penman–Monteith formulations forced by reanalysis data and ESM projections, we found that uncorrected PET strongly reflected land–atmosphere feedbacks, leading to pronounced negative P–PET correlations (-0.45 ± 0.29; mean ± s.d.). When PET was thermodynamically deflated, this dependence was largely removed (-0.02 ± 0.42), restoring consistency with the theoretical basis of Budyko-type diagnostics. This structural correction reduced inflation of the aridity index and substantially moderated projected evapotranspiration (ET) trends. Under a business-as-usual scenario, the trend of Budyko-based ET from uncorrected PET (+0.61 mm yr-2) exceeded that of CMIP6 ensemble mean (+0.28 mm yr-2) by more than a factor of two. CEP-deflated PET narrowed this discrepancy (+0.39 mm yr-2), while additional physiological adjustments provided comparatively smaller improvements. We suggest that violations of structural assumptions, rather than missing physiological processes alone, can play a central role in the divergence between offline aridity diagnostics and ESM hydrological projections.

Acknowledgement: This work was jointly supported by the National Research Foundation of Korea (NRF) grants funded by the Korea government (MSIT) (RS-2025-16070291 & RS-2024-00416443).

How to cite: Kim, D. and Choi, M.: Why offline aridity diagnostics overestimate future drying: the role of feedback-inflated evaporative demand, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6189, https://doi.org/10.5194/egusphere-egu26-6189, 2026.

EGU26-6930 | ECS | Posters on site | NP1.2

Barotropic waves in a sloping two- and multiple-basin Arctic ocean model 

Michael Duc Tung Nguyen and Edward Johnson

Large-scale barotropic flow in the Arctic Ocean is strongly steered by the seafloor topography, yet how this geometry constrains free modes and facilitates inter-basin interactions remains unclear. Free modes conserve potential vorticity and at high latitudes the circulation pathway is enclosed by its sloping two-basin geometry. We begin by presenting a simple two-basin model, representing the Canadian and Eurasian basin respectively, with sloping boundaries and flat bottoms to explore simplified Arctic flow behaviour. Topographic Rossby waves are analytically obtained and the two basins are linked together via a mode-matching framework. We show free modes are tightly constrained to geometry, with basin-trapped dipole wave modes only emerging in certain geometric parameters. We then extend this to a more realistic, multiple-basin Arctic Ocean model that include the Nordic seas, and demonstrate the transmission and exchange of these topographic waves across these multiple sloping basins.

How to cite: Nguyen, M. D. T. and Johnson, E.: Barotropic waves in a sloping two- and multiple-basin Arctic ocean model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6930, https://doi.org/10.5194/egusphere-egu26-6930, 2026.

EGU26-7143 | ECS | Posters on site | NP1.2

Jax-esm: a differentiable coupler for jax-based Earth system models 

Tien-Yiao Hsu, Duncan Watson-Parris, and Georg Feulner

The differentiability of numerical climate models exhibits  many advantages over non-differentiable models. Differentiable climate models would be able to optimize parameters and quickly solve for climate equilibrium. They can also be used to find unstable climate equilibrium states that are impossible to identify in time-forwarding models. Differentiability also enables sensitivity studies, such as the impact of initial conditions on predictions, which is the key concept in the 4-dimensional variational method. Finally, differentiable ability also integrates well with the trending data-driven artificial intelligence model, such as NeuralGCM.  

Currently, physics-based differentiable coupled climate models are still rare. Some existing ones include: ECMWF Integrated Forecasting System (ECMWF-IFS) and Coupled Ocean/Atmosphere Mesoscale Prediction System (COAMPS). The high scientific value of such a tool warrants development of further differentiable modelling systems.

In this work, we present jax-esm, a differentiable coupler for models written in Python with the JAX framework. JAX is a Python library developed by Google that builds on NumPy and adds automatic differentiation and just-in-time (JIT) compilation. It has been used to develop atmospheric models such as NeuralGCM and jax-gcm. In this example, we couple jax-gcm, a JAX-based atmosphere intermediate model, to a slab ocean model. We demonstrate the optimization of ocean mixed-layer depth and solving for climate equilibrium through differentiability.

How to cite: Hsu, T.-Y., Watson-Parris, D., and Feulner, G.: Jax-esm: a differentiable coupler for jax-based Earth system models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7143, https://doi.org/10.5194/egusphere-egu26-7143, 2026.

EGU26-7983 | ECS | Posters on site | NP1.2

Multi-stability of the Global Overturning Circulation: A Conceptual Approach 

Elian Vanderborght and Henk Dijkstra

The Global Overturning Circulation (GOC) is characterized by deep water formation in the subpolar North Atlantic, which feeds the southward-flowing branch of the Atlantic Meridional Overturning Circulation (AMOC). In contrast, the North Pacific lacks deep water formation and therefore does not host an analogous Pacific Meridional Overturning Circulation (PMOC). Proxy records, however, indicate that this asymmetric pattern of deep water formation has varied in the past, suggesting that a PMOC likely existed during earlier climate states. Recent studies further show that the development of a PMOC influences the future weakening of the AMOC: climate models that develop a PMOC in response to warming exhibit a stronger decline in AMOC strength. It therefore becomes important to understand under what circumstances a PMOC is likely to develop.

Here, we extend the pycnocline model of Gnanadesikan (1999) to a two-basin configuration, consisting of a narrow basin representing the Atlantic and a wide basin representing the Pacific. By including salinity as a prognostic variable, we find that this two-basin box model may exhibit three distinct overturning states under identical, longitudinally symmetric forcing: (1) an active narrow-basin sinking state, (2) an active wide-basin sinking state, and (3) a state with active sinking in both basins. Overturning states confined to a single basin are stabilized by the salt-advection feedback, whereas the state with sinking in both basins is maintained by a meridional temperature contrast. We find that this latter state becomes the preferred equilibrium when the interhemispheric temperature contrast increases, the northern gyre transport strengthens, and the hydrological cycle weakens. Moreover, we show that this state is more sensitive to high-latitude freshwater fluxes, indicating that a transition to such a state would enhance the projected future weakening of the AMOC. We verify these findings in an uncoupled global circulation model (MITgcm) with a simplified model geometry.

How to cite: Vanderborght, E. and Dijkstra, H.: Multi-stability of the Global Overturning Circulation: A Conceptual Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7983, https://doi.org/10.5194/egusphere-egu26-7983, 2026.

EGU26-8370 | ECS | Posters on site | NP1.2

Quantifying AMOC Uncertainty in European Climate Damage Projections 

Felix Schaumann

Estimates of economic damages from climate change in Europe depend on temperature projections, and they are thereby subject to scenario uncertainty and model uncertainty, as well as damage function uncertainty. An additional, often implicit source of uncertainty is the projected, yet poorly constrained, weakening of the Atlantic Meridional Overturning Circulation (AMOC), which would lower European temperatures. Here, I explicitly quantify the contribution of AMOC uncertainty to total damage uncertainty, with AMOC uncertainty comprising uncertainty about future AMOC developments as well as uncertainty about the cooling pattern that would follow an AMOC weakening. I combine a newly developed pattern-scaling-type emulator of the European cooling response to AMOC weakening — calibrated for different Earth system models (ESMs) — with temperature projections from multiple ESMs and emissions scenarios, alongside several damage functions. This allows me to decompose the total uncertainty in European economic damages into different drivers and estimate the share attributable to the behaviour of the AMOC.

How to cite: Schaumann, F.: Quantifying AMOC Uncertainty in European Climate Damage Projections, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8370, https://doi.org/10.5194/egusphere-egu26-8370, 2026.

The history of climate modelling is one of increasing complexity and increasing resolution, driven by and constrained by the available computational capacity. These models are widely used, directly and indirectly, to support policy and adaptation decisions across society. They are also used in academic studies across a range of disciplines to study the response of the climate system to future atmospheric greenhouse gas concentrations on multi-decadal timescales. These are extrapolatory endeavours in a non-stationary system without possibility of relevant verification.

There has been much research on individual and multi-model analyses in this context. Here I will instead discuss how the targets of our endeavours (particularly the support of societal decisions) demands a rethinking of our modelling activities. I will highlight the need to reflect on the minimum requirements for ensemble size and ensemble variety, and the role of a hierarchy of models in providing the best possible information to stakeholders across society.

These issues will be discussed in the light of a recent meeting on the foundations of climate change science attended by over 70 researchers across a variety of disciplines. The meeting was entitled “How to spend 15 billion dollars?: A workshop on how to make climate change modelling more robust and more useful to society.” It gathered expertise from disciplines as diverse as earth system modelling, integrated assessment modelling, philosophy, economics, maths, statistics and finance.

Here I will present the key messages coming out of this meeting alongside the themes presented in a recent essay on the subject, “A Model of Catastrophe”[1].

[1] Stainforth, D.A., “A Model of Catastrophe”, Aeon.co, 2025 (https://aeon.co/essays/todays-complex-climate-models-arent-equivalent-to-reality)

How to cite: Stainforth, D.: Designing Climate Change Modelling to Support Societal Decisions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8434, https://doi.org/10.5194/egusphere-egu26-8434, 2026.

EGU26-9869 | Orals | NP1.2

Cascaded score-based emulation of Earth system models for impact evaluation with SCALES-MESH  

Verena Kain, Niklas Schwind, Annika Högner, Assaf Shmuel, Alexander Nauels, Zebedee Nicholls, Marco Zecchetto, and Carl-Friedrich Schleussner

Today's climate adaptation and mitigation planning tasks require rapid access to large ensembles of climate projections for a wide range of emissions scenarios, including overshoot scenarios. While Earth system models (ESMs) provide physically consistent projections, their high computational cost limits scenario exploration. Climate emulators -  statistical or machine-learning-based models trained on ESM data to generate data replicating the ESMs behaviour for a multitude of emissions scenarios - are therefore proposed to deliver these projections efficiently. Here we present the novel modular SCALES–MESH emulator framework, combining physics-based regional projections with AI downscaling capabilities. The SCALES module translates projections of global mean surface air temperature into regional surface air temperature projections aggregated over the AR6-IPCC regions, while the MESH module performs spatio-temporal downscaling to gridded fields using a conditional score-based generative model. MESH is trained on multiple datasets and evaluated against parent ESMs using spatial, temporal, and distributional diagnostics. Results show that the emulator captures regional patterns, temporal variability, and probability distributions of emulated climate variables, including during warming and cooling phases of overshoot scenarios. We further demonstrate the potential for transfer learning across ESMs, pointing toward scalable multi-model and resolution-agnostic emulation. Together, SCALES–MESH enables rapid, flexible, and physically grounded exploration of climate futures, supporting decision-relevant climate risk assessment at unprecedented scope.

How to cite: Kain, V., Schwind, N., Högner, A., Shmuel, A., Nauels, A., Nicholls, Z., Zecchetto, M., and Schleussner, C.-F.: Cascaded score-based emulation of Earth system models for impact evaluation with SCALES-MESH , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9869, https://doi.org/10.5194/egusphere-egu26-9869, 2026.

EGU26-12377 | ECS | Orals | NP1.2

Conditions for instability in the climate–carbon cycle system 

Joseph Clarke, Chris Huntingford, Paul Ritchie, Rebecca Varney, Mark Williamson, and Peter Cox

The climate and carbon cycle interact in multiple ways. An increase in carbon dioxide in the atmosphere warms the climate through the greenhouse effect, but also leads to uptake of CO2 by the land and ocean sink, a negative feedback. However, the warming associated with a CO 2 increase is also expected to suppress carbon uptake, a positive feedback. This study addresses the question: “under what circumstances could the climate–carbon cycle system become unstable?” It uses both a reduced form model of the climate–carbon cycle system as well as the complex land model JULES, combined with linear stability theory, to show that: (i) the key destabilising loop involves the increase in soil respiration with temperature; (ii) the climate–carbon system can become unstable if either the climate sensitivity to CO2 or the sensitivity of soil respiration to temperature is large, and (iii) the climate–carbon system is stabilized by land and ocean carbon sinks that increase with atmospheric CO2 , with CO2-fertilization of plant photosynthesis playing a key role. For central estimates of key parameters, the critical equilibrium climate sensitivity (ECS) that would lead to instability at current atmospheric CO2 lies between about 11K (for large CO2 fertilization) and 6K (for no CO2 fertilization). Given the apparent stability of the climate–carbon cycle, we can view these parameter combinations as implausible. The latter value is close to the highest ECS values amongst the latest Earth Systems Models. We find that the stability of the climate–carbon system increases with atmospheric CO2 , such that the glacial CO2 concentration of 190 ppmv would be unstable even for ECS greater than around 4.5 K in the absence of CO2 fertilization of land photosynthesis.

How to cite: Clarke, J., Huntingford, C., Ritchie, P., Varney, R., Williamson, M., and Cox, P.: Conditions for instability in the climate–carbon cycle system, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12377, https://doi.org/10.5194/egusphere-egu26-12377, 2026.

EGU26-12408 | ECS | Posters on site | NP1.2

Revealing Probabilistic Patterns of Climate Extremes and Impacts Through Emulator-Based Risk Analysis 

Lorenzo Pierini, Chahan Kropf, Lukas Gudmundsson, Sonia I. Seneviratne, and David N. Bresch

Traditional earth system model ensembles provide valuable information on climate extremes. However, their limited size often underrepresents rare high-impact events, restricting the ability to explore extreme outcomes and large-scale anomaly patterns. Using the climate emulator MESMER, trained on CMIP6 models, together with the risk assessment platform CLIMADA, we assess population exposure to annual maximum daily temperatures and asset exposure to annual maximum daily precipitation.

MESMER generates virtually unlimited, spatially explicit, global climate realizations for any scenario defined by emission or global-mean-temperature trajectories. This allows us to characterize the spread of potential outcomes and associated spatial patterns, identify rare high-impact realizations, compare results with standard CMIP6 ensembles, or explore custom scenarios beyond existing model experiments.

We illustrate spatial and temporal patterns of exposure for temperature and precipitation extremes, highlighting contrasting regional responses and how highly impactful outcomes can emerge from climate variability.



How to cite: Pierini, L., Kropf, C., Gudmundsson, L., Seneviratne, S. I., and Bresch, D. N.: Revealing Probabilistic Patterns of Climate Extremes and Impacts Through Emulator-Based Risk Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12408, https://doi.org/10.5194/egusphere-egu26-12408, 2026.

EGU26-12585 | Posters on site | NP1.2

Parsimonious models emulating millennium-long Earth system model simulations 

Kristoffer Rypdal

Parsimonious emulator models (PEMs) trained on Earth system models (ESMs) can be very useful when information  about global quantities like global mean surface temperature (GMST) and ocean heat content (OHC) are sought. Here, I use data over several millennia from ESM runs extracted from the LongRunMip repository to construct and test PEMs for GMST and net incoming radiation flux.

For the  GMST, I consider a linear impulse response in the form of a superposition of three decaying exponentials, comprising three weight coefficients and three characteristic decay times to be estimated by least square fitting to ESM runs with abrupt step function forcing. The model fit is good on all time scales, and the fitted model seems to perform even better for smoother forcing scenarios. This sugggests that the six model parameters represent essential features of each ESM.

Data for radiation flux, and its decomposition in longwave and reflected shortwave, are combined with GMST to produce Gregory plots. By fitting parabolic curves to these plots, I obtain a simple analytic expression for the evolution of the feedback parameter λt), the radiation fluxes, and the resulting increase in OHC.

From these PEMs we can easily compare the global performance of different ESMs under different forcing scenarios. For instance, a comparison of the GISS-E2-R and CESM104 models exhibit equilibrium climate sensitivities (ECSs) of 3.4  and 2.4 K, respectively. The main reason for the difference is very different albedo feedbacks in the two models. Resulting total feedback parameter  λ(t) drops from 2.1 to 1.0 Wm-2 K-1 in GISS-E2-R and from 1.4 to 0.6 Wm-2 K-1 in CESM104. The OHC grows at nearly the same rate in the two models during the first millenium, but GISS saturates earlier and at lower final OHC.

How to cite: Rypdal, K.: Parsimonious models emulating millennium-long Earth system model simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12585, https://doi.org/10.5194/egusphere-egu26-12585, 2026.

EGU26-12666 | Orals | NP1.2

Exploring state dependence of the climate response to radiative forcing using two idealized coupled climate models 

Christopher Pitt Wolfe, Youwei Ma, Anna Katavouta, Kevin Reed, and Richard Williams

Studies of climate sensitivity and feedbacks typically employ a suite of models with similar base climates but different model physics. Such an approach is useful for uncovering how changes to physical processes affect the climate response to changes in radiative forcing, but obscures the dependence of the climate response on the initial state of the climate itself. In order to better understand this dependence, we study the response to radiative forcing of two nearly identical configurations of the Community Earth System Model (CESM) with production-grade physics and resolutions that have dramatically different climates. The first, called Aqua, is completely covered with a uniform-depth ocean except for two 10º-wide polar continents to avoid the polar singularities in the ocean model. The second, Ridge, is identical to Aqua except for the presence of a thin ridge continent connecting the two polar caps. The ridge supports gyres in the ocean and leads to a warm, ice-free climate resembling a global Pacific Ocean, with a warm pool and cold tongue in the tropical ocean connected by a Walker circulation in the atmosphere. In contrast, the mean climate of Aqua is zonally symmetric and dominated by a global cold belt in the ocean driven by vigorous equatorial upwelling. The lack of gyres leads to a deep oceanic thermocline and reduces meridional heat transport, which allows for the development of persistent sea ice at high latitudes.

These two mean climates are perturbed by increasing atmospheric CO2 concentration at a rate of 1% per year until quadrupling. Aqua initially warms more slowly than Ridge, with the transient climate response (TCR) at doubling 23% smaller for Aqua than Ridge. After doubling, however, Aqua begins to warm faster than Ridge and Aqua’s global mean temperature surpasses Ridge’s at quadrupling. A linear feedback analysis is used to gain insight into the time-evolving responses of these two configurations to increased CO2 concentration. At all stages, Aqua’s net top-of-the-atmosphere heating is greater than Ridge’s. At early times, this is due to high clouds replacing low clouds in Aqua’s high latitudes, but decreasing surface albedo due to sea-ice loss eventually becomes a dominant factor. Aqua’s deep thermocline supports a higher ocean heat uptake (OHU) efficiency relative to Ridge that initially offsets these positive feedbacks and results in Aqua’s lower TCR. As CO2 concentration approaches quadrupling, the combined effects of declining OHU efficiency and a strengthening ice-albedo feedback drive Aqua’s warming to temperatures compatible to Ridge. In the century following quadrupling, Aqua warms several Kelvin more than Ridge.

These idealized systems can shed light on the fundamental aspects of Earth’s climate system—such as how the response to radiative forcing depends on the base climate—that might be obscured in more complex configurations.



How to cite: Pitt Wolfe, C., Ma, Y., Katavouta, A., Reed, K., and Williams, R.: Exploring state dependence of the climate response to radiative forcing using two idealized coupled climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12666, https://doi.org/10.5194/egusphere-egu26-12666, 2026.

EGU26-13950 | Orals | NP1.2 | Highlight

Understanding regional discrepancies using the climate model hierarchy 

Tiffany Shaw and Joonsuk Kang

As Earth warms, regional climate signals are accumulating. Some signals, for example, land warming more than the ocean and the Arctic warming the most, were expected and successfully predicted. Underlying this success was the application of physical laws across a climate model hierarchy under the assumption that large and small spatial scales are well separated. With additional warming, however, discrepancies between real-world signals and model predictions are accumulating, especially at regional scales. In this talk, we will highlight the emerging list of model-observation discrepancies in historical trends. We demonstrate how the climate model hierarchy can be used to understand the physical processes underlying these discrepancies. We argue that progress can be made by filling gaps in the hierarchy and making more process-informed observations.

How to cite: Shaw, T. and Kang, J.: Understanding regional discrepancies using the climate model hierarchy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13950, https://doi.org/10.5194/egusphere-egu26-13950, 2026.

EGU26-14266 | ECS | Orals | NP1.2

Rate-dependent Tipping of the AMOC under CO2 increase in an Intermediate Complexity Model 

Sjoerd Terpstra, Swinda Falkena, Robbin Bastiaansen, and Anna von der Heydt

The stability of the Atlantic Meridional Overturning Circulation (AMOC) under future climate change remains uncertain. While most climate models across the model hierarchy project a weakening or collapse under freshwater forcing, transient simulations under increasing CO2 levels also commonly show a weakening or even a collapse of the AMOC. However, longer equilibrium experiments---primarily conducted with lower-complexity models due to computational costs---show more varied responses to CO2 forcing. While most models show an initial weakening of the AMOC, some models equilibrate to a weak AMOC state only at very high CO2 levels, while others equilibrate to a stronger-than-present AMOC. One such model is the intermediate complexity model CLIMBER-X, which (in equilibrium) shows that the AMOC strengthens until at least 16 times preindustrial CO2 levels are reached. However, during the transient phase of increasing CO2, the AMOC weakens. This suggests that the AMOC's transient response may differ from its equilibrium behavior. This raises the question: can the AMOC collapse under rapid and high CO2 increase, even if a stable equilibrium state exists? 

We show that the AMOC exhibits rate-dependent tipping; when CO2 increases fast enough and reaches sufficiently high levels, the AMOC can fully collapse. This occurs under very high forcing, starting from 7 times preindustrial CO2 levels and a rate of 2.0% ppm/yr CO2 increase. This collapse occurs despite the existence of a stable AMOC at equilibrium. By examining the physical processes through which the collapse occurs, we contribute to the understanding of the AMOC response in a warming climate. By also incorporating freshwater forcing, we assess the risks of rapid warming on the AMOC stability. Our results show that even models with a stable equilibrium AMOC under high CO2 levels can experience weakening during the transient phase or even collapse. This highlights the need to assess both the rate and magnitude of CO2 forcing when assessing the stability of the AMOC. While this effect occurs at very high CO2 levels in CLIMBER-X, the role of the rate of CO2 increase may become relevant at lower CO2 levels when combined with freshwater forcing. Our findings demonstrate that the AMOC can undergo rate-dependent tipping under rapid and high CO2increase, even if a stable AMOC exists at very high CO2 levels.

How to cite: Terpstra, S., Falkena, S., Bastiaansen, R., and von der Heydt, A.: Rate-dependent Tipping of the AMOC under CO2 increase in an Intermediate Complexity Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14266, https://doi.org/10.5194/egusphere-egu26-14266, 2026.

EGU26-14741 | Posters on site | NP1.2

Coupled ESM-IAM Emulator: Exploring Uncertainties in Temperature Target Pathways 

Katsumasa Tanaka, Xiong Weiwei, Myles Allen, Michelle Cain, Stuart Jenkins, Camilla Mathison, Vikas Patel, Chris Smith, and Kaoru Tachiiri

Integrating physical, socio-economic, and technological perspectives is indispensable for addressing climate mitigation challenges. While directly coupling state-of-the-art Earth System Models (ESMs) and Integrated Assessment Models (IAMs) offers a way to explore feedbacks between these domains, doing so with full-complexity models remains computationally prohibitive. This is particularly true for cost-effective intertemporal optimization IAMs due to fundamental operational differences: while ESMs perform forward simulations, such IAMs optimize over time. Consequently, direct coupling would require numerous computationally intensive iterations to converge, a complication further compounded by the stochastic nature of ESMs.

To overcome the barriers to coupling ESMs and IAMs, we employ their reduced-complexity representations (i.e., emulators). We couple an IAM emulator representing 9 distinct IAMs (Xiong et al. 2025) with an ESM emulator, FaIR, representing 66 ESM configurations (Smith et al. 2024a). Using this coupled ESM-IAM emulator framework in an optimization setting, we calculate cost-effective pathways that achieve the temperature targets of the Paris Agreement with and without overshoot.

Our preliminary results indicate that the uncertainty ranges for such pathways are significantly larger than previously estimated. Our results also have implications for target setting; we show how pathways differ when IAMs optimize directly for a temperature target – a capability IAMs traditionally lack. Instead, IAMs typically rely on temperature proxies, such as carbon budgets (or their corresponding carbon price pathways), which do not necessarily provide an accurate representation of the temperature target. Furthermore, this study offers advanced insights into the dynamics of climate-economy interactions, providing a roadmap for future efforts to couple full-complexity models.

 

References

Xiong, W., Tanaka, K., Ciais, P., Johansson, D. J. A., & Lehtveer, M. (2025). emIAM v1.0: an emulator for integrated assessment models using marginal abatement cost curves. Geosci. Model Dev., 18(5), 1575-1612. doi:10.5194/gmd-18-1575-2025

Smith, C., Cummins, D. P., Fredriksen, H. B., Nicholls, Z., Meinshausen, M., Allen, M., . . . Partanen, A. I. (2024). fair-calibrate v1.4.1: calibration, constraining, and validation of the FaIR simple climate model for reliable future climate projections. Geosci. Model Dev., 17(23), 8569-8592. doi:10.5194/gmd-17-8569-2024

How to cite: Tanaka, K., Weiwei, X., Allen, M., Cain, M., Jenkins, S., Mathison, C., Patel, V., Smith, C., and Tachiiri, K.: Coupled ESM-IAM Emulator: Exploring Uncertainties in Temperature Target Pathways, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14741, https://doi.org/10.5194/egusphere-egu26-14741, 2026.

EGU26-15472 | ECS | Posters on site | NP1.2

Low Uncertainty Regional Climate Projections without Irrelevant Weather Details 

Yifan Wang, Shaun Lovejoy, Dustin Lebiadowski, and Dave Clarke

Uncertainties in conventional (GCM) climate models, defined as the structural spread among com-
peting models, have increased for the first time in the latest AR6 report despite an exponential increase
in the modern computation power. The root problem is that these models are based in the weather
regime, that is, they spend unnecessary effort in calculating irrelevant weather details. This project
aims to produce precise regional projection using the Half Order Energy Balance Equation (HEBE): a
half order fractional derivative generalization of the standard Energy Balance Equation (EBE). HEBE
has the advantage of being a direct consequence of the continuum heat equation combined with energy-
conserving surface boundary conditions. A previous paper used Fractional EBE (FEBE) to model Earth
climate projections through 2100 on a global scale, and it yields significantly smaller uncertainty com-
pared to the CMIP6 MME. This project builds on a similar methodology, enhancing climate projection
with additional regional details and upgraded precision. The current results show that the parametric
uncertainty in HEBE’s temperature response is smaller than the internal variability at most locations,
at the exceptions of the high memory deep ocean regions near Pacific. HEBE’s regional hindcast ac-
curately reproduces ERA5 2mT series’ deterministic and stochastic patterns of regional temperature.
The global hindcast is also validated by various reanalysis datasets and instrumental records. The
direct year to year relative uncertainty (ratio between 90% confidence interval and best estimate) is
stable across time and marker scenarios, with most regions projecting values below 0.5 by 2100. On a
global scale, the parametric uncertainty in HEBE’s response temperature is negligible (±0.03K by 2100
using the SSP2-4.5 marker scenario). This effectively shows that HEBE’s projection is more precise
than its competitors even without taking period averages. The exceedingly low global uncertainty was
constrained by the large amount of regional information when taking the global averages. It should be
noted that the cited parametric uncertainty does not take into account systematic biases in HEBE and
in the input datasets. The most important source should be any errors in the forcings, especially con-
cerning aerosols. HEBE aims to provide a compelling and physically grounded alternative to complex
deterministic multi-model ensembles, offering a more precise, efficient, and interpretable means of pro-
jecting regional climate changes in the coming century. This positions it as a potentially valuable tool
for policy-relevant projections and adaptation planning, thereby showing the pertinency of fractional
derivative and Bayesian framework in atmospheric sciences.

How to cite: Wang, Y., Lovejoy, S., Lebiadowski, D., and Clarke, D.: Low Uncertainty Regional Climate Projections without Irrelevant Weather Details, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15472, https://doi.org/10.5194/egusphere-egu26-15472, 2026.

EGU26-16369 | Posters on site | NP1.2

The future is in the past? A flexible resampling approach to generate multivariate time series 

Michael Lehning, Tatjana Milojevic, and Pauline Rivoire

Synthetic time series generation is an essential tool for robustly exploring different climate scenarios and their impacts. While sophisticated generation methods have been developed in the past, they often rely on physical and statistical assumptions and require extensive data for calibration and parameter estimation. We propose a straightforward method for time series generation based on constrained sampling of observations. This approach preserves the physical consistency between variables and maintains the short temporal structure present in the observation. We apply this procedure to generate temperature, precipitation, incoming solar radiation, and wind speed time series sampled from meteorological station observations. We obtain different sets of synthetic time series by constraining the mean temperature according to future scenarios provided by climate model projections. We show that the sampled time series preserve the multivariate dependence structure observed in both historical data and climate projections. While, by design, the method does not generate daily values beyond the observed range, it can simulate multi-day extremes that exceed those in the observational record, such as longer heatwaves. The approach is flexible and can be applied to other variables with other constraints, provided that a sufficiently long observational time series is available and the constraints are compatible with the observed data. The generation procedure may thus prove useful for studying potential future extremes and help in general downscaling tasks.

How to cite: Lehning, M., Milojevic, T., and Rivoire, P.: The future is in the past? A flexible resampling approach to generate multivariate time series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16369, https://doi.org/10.5194/egusphere-egu26-16369, 2026.

Reservoirs are increasingly recognized as significant sources of greenhouse gas (GHG) emissions, yet their future emissions under climate change remain poorly quantified. This study evaluates the impact of climate change on net GHG emissions from Feitsui Reservoir, a major water supply reservoir in northern Taiwan, using an integrated modeling approach.

We utilized the multisite Weather Generator (multiWG) to generate future climate projections for three Shared Socioeconomic Pathways (SSP126, SSP245, SSP585) across four 20-year periods (2021-2040, 2041-2060, 2061-2080, 2081-2100), with 1995-2014 as the baseline. A Random Forest model (NSE = 0.8637) was trained to predict reservoir inflow based on temperature and precipitation data. These inflows were input into the G-RES model to calculate net GHG emissions in CO₂-equivalent units, including contributions from both CO₂ and CH₄.

Results reveal that reservoir GHG emissions will increase under all climate scenarios, with magnitude strongly dependent on emission pathways. Under the low-emission scenario (SSP126), emissions increase by 5.2-8.8% across all periods. The intermediate scenario (SSP245) shows moderate increases of 5.4-18.4%. The high-emission scenario (SSP585) demonstrates dramatic escalation, particularly in the late century (2081-2100), where emissions reach 1259.6 gCO₂e/m²/yr—a 45.8% increase. These findings underscore the critical need to consider climate impacts in reservoir management and carbon accounting frameworks.

How to cite: Yeh, F.-W. and Tung, C.-P.: Assessing Climate-Driven Greenhouse Gas Emissions from Feitsui Reservoir Using G-RES Under Multiple SSP Scenarios, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16498, https://doi.org/10.5194/egusphere-egu26-16498, 2026.

EGU26-16683 | Orals | NP1.2

Combining emulators and demographics: Building a flexible toolkit for lifetime exposure assessments 

Quentin Lejeune, Rosa Pietroiusti, Amaury Laridon, Niklas Schwind, Carl-Friedrich Schleussner, and Wim Thiery

Across the globe, today’s young generations will be more frequently exposed to climate extremes over their lifetime than earlier generations. Previous work has established this finding by combining simulations of historical and projected trends in climate extremes together with data on past and future demographic changes (Thiery et al. 2021, Grant et al. 2025). However, it has so far focused on a limited set of climate extreme indicators, using climate (impact) simulations from ISIMIP2 and demographics datasets that are now outdated, and did not fully assess uncertainty across the climate impact modelling chain. 

 

We now build on this existing lifetime exposure framework and combine it with a chain of emulators constituted of a Simple Climate Model (SCM) and the Rapid Impact Model Emulator Extended (RIME-X, Schwind et al., submitted). RIME-X can translate the GMT distributions generated by an SCM for a given emission scenario into spatially explicit distributions of climate or climate impact indicators. It has already been used to produce projections for 40+ indicators derived from ISIMIP3 and other climate model simulations, and this list can be extended to further indicators whose evolution predominantly depends on the level of global warming and for which historical and future simulations are available.   

 

We also update the lifetime exposure framework to consider more recent demographic data, and package it into a GitHub repository called dem4cli (short for ‘demographics for climate’) that will be made publicly available. We use spatially explicit population reconstructions and projections from the COMPASS project, and national-level life expectancy and cohort size estimates and projections from UNWPP2024.  

 

This work delivers more robust calculations of lifetime exposure to changes in extremes or climate impacts, by leveraging the ability of the SCM-RIME-X emulator chain to represent both their forced response to emissions as well as the combined uncertainty arising from the GMT response to emissions, the local climate response to global warming, and interannual variability, in combination with updated demographic data. This new framework is designed to generate such policy-relevant information in a more flexible and systematic manner, as it can in theory be applied to any available emission or GMT trajectories, and extended to a broad range of climate hazards.

Thiery, W. et al. Intergenerational inequities in exposure to climate extremes. Science 374, 158–160 (2021) 

Grant, L., Vanderkelen, I., Gudmundsson, L. et al. Global emergence of unprecedented lifetime exposure to climate extremes. Nature 641, 374–379 (2025) 

Schwind et al. RIME-X v1.0: Combining Simple Climate Models, Earth System Models, and Climate Impact Models into a Unified Statistical Emulator for Regional Climate Indicators. Geoscientific Model Development (submitted) 

How to cite: Lejeune, Q., Pietroiusti, R., Laridon, A., Schwind, N., Schleussner, C.-F., and Thiery, W.: Combining emulators and demographics: Building a flexible toolkit for lifetime exposure assessments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16683, https://doi.org/10.5194/egusphere-egu26-16683, 2026.

EGU26-16747 | ECS | Orals | NP1.2

The effect of freshwater biases on AMOC stability across the model complexity spectrum 

Amber Boot and Henk Dijkstra

A collapse of the Atlantic Meridional Overturning Circulation (AMOC) would have strong consequences for the global climate system.  Assessing whether the AMOC will collapse in the future is difficult since current Earth System Models (ESMs) have biases. An earlier study using an intermediate complexity Earth system model (EMIC) showed the potential effect of freshwater biases on AMOC stability.  However, the used model has a limited ocean model with respect to the used  resolution and processes represented compared to ESMs. Here, we supplement the EMIC simulations with simulations of an ocean-only model using the same resolution as is typically used in ESMs. This allows us to study the effect of ocean resolution on the physical mechanism controlling the effect of freshwater biases on AMOC stability. We find that both the intermediate complexity and the ocean-only model behave qualitatively similar. In both models freshwater biases influence AMOC stability where negative (positive) biases in the Indian Ocean tend to stabilize (destabilize) the AMOC, whereas the opposite applies to biases in the Atlantic Ocean. Based on the freshwater biases present in most ESMs, our results suggest that most ESMs have a too stable AMOC and might therefore underestimate the probability of an AMOC collapse under future emission scenarios.

How to cite: Boot, A. and Dijkstra, H.: The effect of freshwater biases on AMOC stability across the model complexity spectrum, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16747, https://doi.org/10.5194/egusphere-egu26-16747, 2026.

EGU26-17291 | ECS | Posters on site | NP1.2

Using Ice Cores and Gaussian Process Emulation to Recover Changes in the Greenland Ice Sheet During the Holocene 

Irene Malmierca Vallet, Louise C. Sime, Jochen Voss, Diego Fasoli, and Kelly Hogan

The shape and extent of the Greenland Ice Sheet (GIS) during the Holocene remain a matter of considerable debate, with existing studies proposing a wide range of reconstructions. In this study, we aim to combine stable water isotopic information from ice cores with outputs from isotope-enabled climate models to investigate this problem. Directly exploring the space of possible ice sheet geometries through numerical simulations is computationally prohibitive. To address this challenge, we plan to develop a Gaussian process emulator that will serve as a statistical surrogate for the full climate model. The emulator will be trained on the results of a limited number of carefully designed simulations and will be used to enable fast, probabilistic predictions of model outputs at untried inputs. The inputs will consist of GIS morphologies, parameterized using a dimension-reduction technique adapted to the spherical geometry of the ice sheet. Using predictions from the emulator, we will explore the range of ice sheet morphologies that are compatible with available ice-core isotope measurements and other complementary observational data, including those collected during recent KANG-GLAC expeditions, with the goal of ultimately reducing uncertainty in reconstructions of Holocene GIS morphology.

How to cite: Malmierca Vallet, I., Sime, L. C., Voss, J., Fasoli, D., and Hogan, K.: Using Ice Cores and Gaussian Process Emulation to Recover Changes in the Greenland Ice Sheet During the Holocene, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17291, https://doi.org/10.5194/egusphere-egu26-17291, 2026.

EGU26-18639 | Posters on site | NP1.2

The compact Earth system model OSCAR v4 

Thomas Gasser, Biqing Zhu, Xinrui Liu, Danni Zhang, Yuqin Lai, and Gaurav Shrivastav

OSCAR is an open-source reduced-complexity Earth system model designed to probabilistically emulate the coupled climate–carbon–chemistry system with low computational cost. Following a preivously published evaluation of OSCAR v3.1 against observations and CMIP6 Earth system models, we present OSCAR v4, which incorporates a range of structural, numerical, and methodological improvements. Key developments include enhanced numerical stability, modularization of the code to allow running submodels independently, revised and streamlined modules, and recalibration using the latest AR6, CMIP6, and TRENDY datasets. Monte Carlo sampling has been improved using continuous probability distributions, and the constraining strategy now leverages Latin-hypercube sampling combined with probability integral transforms to provide more robust probabilistic ensembles compatible with observations. Alongside core model improvements, OSCAR v4 will introduce a suite of user-oriented functionalities and a full online documentation, facilitating broader adoption and reproducibility.

We illustrate the performance of OSCAR v4 through participation in the Reduced Complexity Model Intercomparison Project (RCMIP) phase 3 exercise. This benchmarking demonstrates the model’s ability to reproduce the spread of global temperature and carbon-cycle responses observed in more complex Earth system models, while providing rapid, policy-relevant probabilistic projections. Given it's level of complexity, OSCAR v4 is positioned as a versatile tool bridging comprehensive Earth system models and the simpler reduced-complexity approaches for large-scale climate assessments.

How to cite: Gasser, T., Zhu, B., Liu, X., Zhang, D., Lai, Y., and Shrivastav, G.: The compact Earth system model OSCAR v4, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18639, https://doi.org/10.5194/egusphere-egu26-18639, 2026.

EGU26-19277 | Orals | NP1.2

From scenarios to impacts – an emulation of regional climate impacts and their uncertainties using the CMIP7 mitigation scenarios    

Daniel Hooke, Camilla Mathison, Eleanor Burke, Chris Jones, Laila Gohar, and Andy Wiltshire

The PRIME (Mathison et al. 2025) framework provides a fast response tool to look at climate impacts for up-to-date mitigation scenarios. PRIME combines the FaIR simple climate model and pattern scaling of Earth System Models (ESMs) with the JULES land surface model to quantify spatially resolved climate impacts. In addition, PRIME samples uncertainty from both the spatial patterns of CMIP6 ESMs and the probabilistic configuration of the latest version of FaIR. 

We present applications of this framework to explore impacts on both the earth system and potential impacts on societies, using new scenarios produced for CMIP7. From an earth system perspective, we use an updated configuration of JULES incorporating permafrost processes and fire to look at the impact of the northern high latitude net ecosystem balance. In terms of societal impacts, we simulate the potential impacts of climate change on agricultural drought of rain fed crops during the growing season. This analysis includes a quantification of the uncertainty derived from the global mean climate response and the spatial responses of ESMs. Results from PRIME will also be part of the FastMIP project. 

How to cite: Hooke, D., Mathison, C., Burke, E., Jones, C., Gohar, L., and Wiltshire, A.: From scenarios to impacts – an emulation of regional climate impacts and their uncertainties using the CMIP7 mitigation scenarios   , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19277, https://doi.org/10.5194/egusphere-egu26-19277, 2026.

EGU26-19612 | ECS | Posters on site | NP1.2

Accounting for Aerosols in Climate Mitigation Pathways 

Tomás Arzola Röber, Thomas Bruckner, and Johannes Quaas

To meet Paris-aligned climate goals and minimize temperature overshoot and its impacts, rapid and deep reductions in greenhouse-gas emissions from fossil-fuel combustion are required. Climate risk projections are strongly affected by uncertainty in anthropogenic aerosol effective radiative forcing (ERF) and by the co-evolution of air-pollutant emissions under decarbonization pathways. Because running large Earth System Model (ESM) ensembles remains computationally expensive for uncertainty quantification and broad policy-scenario exploration, reduced-complexity climate emulators are needed for efficient, transparent, and observation-connected assessments.

Here we develop an aerosol extension to the simple climate model (SCM) FaIR that emulates aerosol ERF from global anomalies in aerosol optical depth (ΔAOD) relative to a pre-industrial baseline for different species. Aerosol ERF is computed using a constrained parameterization that separates aerosol–radiation and aerosol–cloud interactions, with key parameters represented probabilistically and constrained by observational and model-based lines of evidence.

To emulate ΔAOD from emissions pathways, we implement an interpretable mapping calibrated to CMIP6 ESM output. An effective linear relationship between emission and burden anomalies is fitted using a single parameter that aggregates yield and lifetime effects. In a second step, we fit an effective optical parameter linking burden perturbations to ΔAOD. This produces model-dependent parameter distributions that enable propagation of both parametric uncertainty and between-model spread. In addition, we implement an integrated-assessment-model-based relationship linking air-pollutant emissions to CO₂ emissions under different air-quality policy stringencies, interpolated into a continuous air-quality parameter suitable for exploring uncertainty and its interaction with decarbonization trajectories.

We perform Monte Carlo ensembles sampling aerosol-ERF parameters, CMIP6-calibrated aerosol–AOD mappings, air-quality policy stringency, and net-zero timing, and evaluate impact-relevant climate risk metrics including peak warming, probability of remaining below 1.5 °C, threshold crossing year, overshoot duration, and warming rates computed over multiple near-term and decadal windows. Preliminary results show strong dependence of peak temperature outcomes on net-zero timing, while threshold-based metrics and warming rates exhibit pronounced sensitivity to air-quality assumptions, consistent with a partial loss of aerosol cooling under stricter pollution controls. Overall, the results indicate non-linear interactions between decarbonization timing, air-quality stringency, and warming-rate responses. The emulator provides a scalable basis for robust climate risk screening and for coupling SCM trajectories to impact assessments.

Keywords: Climate Change, Mitigation, Aerosols, Effective Radiative Forcing, Climate Emulators, Climate Modeling, CMIP6 Calibration, Air-quality Policy, Overshoot

How to cite: Arzola Röber, T., Bruckner, T., and Quaas, J.: Accounting for Aerosols in Climate Mitigation Pathways, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19612, https://doi.org/10.5194/egusphere-egu26-19612, 2026.

EGU26-20117 | Posters on site | NP1.2

Applying GWP* to Long-Term Climate Pathways and Fluorinated Gases 

Michelle Cain, Vikas Patel, Matteo Mastropierro, Katsumasa Tanaka, Stuart Jenkins, and Myles Allen

Greenhouse gas emission metrics are widely used for comparing climate impacts of different gases and for guiding mitigation policy. Conventional metrics such as GWP100 perform well for representing the warming effects of long-lived gases which behave like CO₂ but poorly for short-lived climate pollutants (SLCPs). Methane (CH4) is the most important SLCP and has been the main focus of alternative metrics. GWP* was developed to more accurately capture impact on global warming, particularly from stable and declining CH4 emissions which are not well served by GWP100. This means that GWP* better connects emissions pathways to long-term temperature targets (Cain et al., 2022). Previous studies optimised GWP* for CH4 for a limited range of scenarios up to 2100. However, future mitigation pathways involve a wider range of gases and transition speeds, overshoot behaviour, and long-term stabilization beyond this period. In addition, highly radiatively efficient fluorinated gases are increasingly important in mitigation strategies yet have not been demonstrated with the GWP* framework. In this study, we systematically test the performance of GWP* across an expanded set of emissions scenarios, including rapid mitigation, delayed action, and prolonged temperature overshoot pathways, and extend the analysis to multi-century time horizons with an optimisation of the flow term of GWP* (Mastropierro et al., 2025). We further develop and evaluate a generalized formulation of GWP* for fluorinated gases with diverse atmospheric lifetimes. The outcomes examine the performance of GWP* under realistic transition pathways and its representation of temperature responses for fluorinated gases. This work supports the development of more physically consistent multi-gas emission metrics for climate targets, carbon budgeting, and policy design, as it is a simple tool to calculate how much global warming is added or avoided by increasing or cutting SLCPs such as F-gases.

Cain, M., Jenkins, S., Allen, M.R., Lynch, J., Frame, D.J., Macey, A.H., Peters, G.P. Methane and the Paris Agreement temperature goals. Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 380 (2022). https://doi.org/10.1098/rsta.2020.0456

Mastropierro, M., Tanaka, K., Melnikova, I. et al. Testing GWP* to quantify non-CO2contributions in the carbon budget framework in overshoot scenarios. npj Clim Atmos Sci 8, 101 (2025). https://doi.org/10.1038/s41612-025-00980-7

How to cite: Cain, M., Patel, V., Mastropierro, M., Tanaka, K., Jenkins, S., and Allen, M.: Applying GWP* to Long-Term Climate Pathways and Fluorinated Gases, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20117, https://doi.org/10.5194/egusphere-egu26-20117, 2026.

EGU26-20145 | Posters on site | NP1.2

Investigating the possibility of rare spontaneous AMOC transitions in the intermediate complexity climate model FAMOUS. 

Jeroen Wouters, Guannan Hu, Jochen Bröcker, and Robin Smith

Earth System Models of Intermediate Complexity (EMICs) allow for fast exploration of large-scale climate dynamics. These models thus enable the development and testing of large-ensemble-based techniques that would be too costly with more realistic climate models.

In this ongoing study we develop a rare event simulation setup to explore the possibility of a spontaneous collapse of the Atlantic Meridional Overturning Circulation (AMOC) in the FAMOUS model. FAMOUS is a low-resolution, coupled atmosphere-ocean general circulation model derived from the UK Met Office’s Unified Model specifically designed for efficient, long-duration and ensemble climate simulations. FAMOUS has previously been used to investigate the hysteresis of the Atlantic Meridional Overturning Circulation under freshwater hosing.

We apply a genealogical particle analysis (GPA) algorithm that is designed to probe the possibility of spontaneous AMOC transitions. The method initiates an ensemble of realisations in the "on"-state of the AMOC and clones ensemble members at regular intervals  that are showing a low AMOC.

Contrary to recent results in another EMIC, a straightforward sampling based on the AMOC indicator does not result in any spontaneous transitions to the AMOC "off"-state. To improve the selection of potentially exceedingly rare trajectories, we therefore investigate statistical methods to identify physical variables that correlate with the state of the AMOC ahead of time, to be used as selection criteria in the GPA algorithm.

How to cite: Wouters, J., Hu, G., Bröcker, J., and Smith, R.: Investigating the possibility of rare spontaneous AMOC transitions in the intermediate complexity climate model FAMOUS., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20145, https://doi.org/10.5194/egusphere-egu26-20145, 2026.

EGU26-20975 | ECS | Posters on site | NP1.2

Modelling Mesoarchaean climate: Economic implications  

Lisa Wasitschek, Hartwig E. Frimmel, Nina Hiby, and Felix Pollinger

The Witwatersrand Basin on the Kaapvaal Craton hosts the world’s largest gold province, with the vast majority of gold concentrated in the 2.90–2.79 Ga Central Rand Group, whereas the slightly older 2.95–2.91 Ga West Rand Group is largely barren despite comparable sedimentary characteristics. This contrast has been attributed to intensified chemical weathering during Central Rand Group times, which promoted enhanced gold mobilisation from the Archaean hinterland. However, the climatic and environmental drivers of this weathering intensification remain poorly constrained. To address this, we investigated Mesoarchaean climate controls using the Planet Simulator (PlaSim), an Earth system model of intermediate complexity. We conducted 140 PlaSim simulations to quantify the climatic sensitivity to atmospheric greenhouse gas concentrations, continental surface area, surface albedo, and land configuration. CO₂-equivalent concentrations (3–30 %), land coverage (8–28 %), and albedo (0.15–0.30) were systematically varied across different land distributions (equatorial, polar and spread over different latitudes).

Next to the well-known effect of global warming under increased greenhouse gas concentrations, our results show that increasing continental area generally results in global cooling due to the higher albedo of land surfaces relative to oceans, particularly when land was concentrated at low latitudes. This cooling effect becomes pronounced once land exceeds approximately 13 % of Earth’s surface. At high latitudes, land has minimal climatic impact because of the low incoming radiation angle that leads to less absorption. Exceptions are noted under conditions of low greenhouse gas concentrations and low surface albedo, at which limited land growth could slightly enhance warming. Among the tested land positions, the scenario with land spread over different latitudes resulted in the highest climate sensitivity.

Overall, our results indicate that land distribution alone was unlikely to have caused global warming during the Mesoarchaean, and this climatic influence was probably dampened by a more rapid carbon cycle at that time. Instead, elevated atmospheric greenhouse gas levels emerge as the dominant driver of warming and enhanced chemical weathering. The climatic transition around ~2.9 Ga may further reflect the emergence of extensive low-albedo mafic or ultramafic surfaces and/or the latitudinal migration of the Kaapvaal Craton into a more radiatively sensitive, low-latitude zone. These combined factors likely contributed to intensified weathering, increased gold leaching, and the gold megaevent responsible for the formation of the Witwatersrand ores.

How to cite: Wasitschek, L., Frimmel, H. E., Hiby, N., and Pollinger, F.: Modelling Mesoarchaean climate: Economic implications , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20975, https://doi.org/10.5194/egusphere-egu26-20975, 2026.

EGU26-21556 | ECS | Posters on site | NP1.2

Surface albedo as a first-order control on Mesoarchaean climate (PlaSim) 

Nina Hiby, Lisa Wasitschek, and Hartwig E. Frimmel

The radiative balance of the early Earth was governed by other boundary conditions than today, including a fainter Sun, elevated greenhouse gas concentrations, and a smaller land surface area. Although the role of atmospheric composition in sustaining habitable surface temperatures during the Mesoarchaean has been extensively investigated, especially to solve the faint young Sun paradox, the climatic impact of land position and distribution under varying albedo remains comparatively underexplored.

We therefore assess how variations in land-surface albedo, land fraction, and land distribution could have modulated Mesoarchaean climate states. Using the Planet Simulator (PlaSim), an intermediate-complexity climate model, we conducted 195 simulations spanning CO₂-equivalent forcing levels of 3–10 % (30,000–100,000 ppm). Land-surface albedo was varied between 0.15 and 0.30, land area between 8 % and 28 %, and idealised land distributions were prescribed, including diagonal, staggered, and mid-latitude configurations. Ocean albedo was held constant at 0.144 to isolate the climatic impact of continental reflectivity.

Across all simulations, global mean temperature responds strongly and non-linearly to both land fraction and land albedo. At low land albedo (0.15) and low to intermediate CO₂-equivalent forcing (3–5 %), increasing land area produces a slight warming trend, despite minimal differences between land and ocean reflectivity. This behaviour indicates that land–ocean contrasts in surface energy partitioning and effective heat capacity can modify global climate even when shortwave albedo contrasts are small. Sensitivity increases abruptly as land albedo rises from 0.20 to 0.25. Beyond this threshold, modest increases in land area result in pronounced global cooling, consistent with a regime shift in the radiative balance. This non-linear response is most prominent at low to intermediate CO₂-equivalent forcing and becomes progressively muted at higher forcing (10 %), where greenhouse effects dampen the temperature response to surface reflectivity changes. The pattern occurs across all land configurations but is amplified when landmasses occupy equatorial to mid-latitudes, where insolation is highest and albedo exerts maximum leverage, whereas high-latitude land has a comparatively weaker effect.

These findings highlight that land surface characteristics such as albedo and distribution were critical for early Earth’s climate. Even under strongly greenhouse-forced atmospheres, surface properties significantly altered the planetary energy budget. Recognising such sensitivities is essential for reconstructing Archaean climate states and assessing the potential for climatic stability under reduced solar luminosity.

How to cite: Hiby, N., Wasitschek, L., and Frimmel, H. E.: Surface albedo as a first-order control on Mesoarchaean climate (PlaSim), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21556, https://doi.org/10.5194/egusphere-egu26-21556, 2026.

EGU26-21970 | ECS | Posters on site | NP1.2

Simulating NAO-driven AMOC collapse in the PlaSim-LSG Climate Model 

Arianna Magagna, Giuseppe Zappa, Matteo Cini, and Susanna Corti

The Atlantic Meridional Overturning Circulation (AMOC) is a critical component of the global climate system and its potential for abrupt collapse represents a significant tipping point. Our project investigates whether a persistent negative phase of the North Atlantic Oscillation (NAO), a dominant mode of atmospheric variability, can induce an AMOC collapse in the absence of external perturbations within the coupled PlaSim-LSG climate model of intermediate complexity. A control simulation establishes a baseline climatology, confirming that NAO variability leads AMOC fluctuations by approximately one year. To overcome the computational limitation of simulating rare events, we implement a rare event algorithm (GKLT) that efficiently biases the model toward trajectories with negative NAO conditions over 125-year simulations. The results reveal a fundamental bistability in the system. While persistent negative NAO forcing can trigger an AMOC collapse, the outcome is probabilistic: out of six independent ensemble simulations, four evolved entirely into a collapsed state (∼ 12 Sv), one remained entirely vigorous (∼ 23 Sv) and one split into both outcomes. A cluster-based analysis traces this divergence to the early amplification of small differences in North Atlantic heat fluxes, convection and sea-ice cover. These findings show that internal atmospheric variability alone can force the AMOC across a tipping point, highlighting the role of internal climate dynamics in shaping climate transitions.

How to cite: Magagna, A., Zappa, G., Cini, M., and Corti, S.: Simulating NAO-driven AMOC collapse in the PlaSim-LSG Climate Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21970, https://doi.org/10.5194/egusphere-egu26-21970, 2026.

EGU26-536 | ECS | Posters on site | PS2.6

The Effects of Impacts on Europa’s Ice Shell Dynamics 

Davide Izzo, Ana-Catalina Plesa, Kaiyi Dai, Kai Wuennemann, and Hauke Hussmann

Jupiter’s moon Europa is one of the prime targets for planetary exploration due to its high astrobiological potential. Its young surface age, on average between ∼40 – 90 Myr old (Bierhaus et al., 2009) suggests that some form of resurfacing has occurred in the past, with impacts being one of several possible triggering mechanisms. Moreover, impacts onto the ice shell of Europa likely have affected the ice shell dynamics leading to a convective state. 

 

Europa’s ice shell thickness is poorly known with literature values ranging from <1 km (Billings et al., 2005) to 90 km (Villela et al., 2020), with recent studies favoring a range of 23 - 47 km (Howell, 2021). Basin and crater shapes provide important information about the ice shell’s thermal state, thickness, and dynamics (conductive vs. convective). A transition in crater morphology for diameters larger than ∼8 km indicates a weak layer at ~7–8 km depth, as inferred from numerical modelling and observational crater-depth studies (Bray et al., 2014; Schenk, 2002). This layer could potentially represent warm convecting ice or the presence of the liquid ocean (e.g., Silber and Johnson, 2017). A recent study about multiring basins on Europa suggests an ice shell thickness larger than 20 km consisting of a 6-8 km conductive layer overlying a warm convecting region (Wakita et al., 2024).

 

Here, we investigate how impacts affect the dynamics of Europa’s ice shell using the geodynamic code GAIA (Hüttig et al., 2013). Impact thermal-induced and compositional anomalies are parameterized using scaling laws (Melosh, 1989). We assume that the water produced as a consequence of the impact process rapidly recrystallizes, but leaves behind a chemical and thermal anomaly in the shallow layers of the ice shell. Our models include a composite rheology (Goldsby & Kohlstedt, 2001), pressure- and temperature-dependent thermal expansivity and thermal conductivity (Feistel & Wagner; Wolfenbarger et al., 2021), and the effects of tidal heating (Tobie et al., 2003). We test scenarios with different impactor sizes (0.5 km - 1.8 km), thermal states at the time of the impact (i.e. cold conductive or warm convective ice shell), and ice shell rheology (via changing the grain size). We vary the chemical density anomalies due to impactor material assuming mixtures of ice, salts, and dust. To this end, we consider the presence of salts in concentrations ranging between that of the Earth's ocean and twice as high. 

 

Our models show that impacts can initiate thermal convection in an otherwise conductive ice shell. The material introduced by impacts may remain trapped in the cold conductive upper layer if no surface mobilization occurs. For large impacts, the impactor material can reach the convective ice layer and become mixed into the ice shell, reaching the ice-ocean boundary.

 

In a future step, we will consider the impact-induced thermal anomalies based on shock physics models instead of scaling laws. We will use the modelled density anomalies associated with thermal and compositional anomalies introduced by impacts to determine their gravity signature that could be potentially detected by Europa Clipper and JUICE.

How to cite: Izzo, D., Plesa, A.-C., Dai, K., Wuennemann, K., and Hussmann, H.: The Effects of Impacts on Europa’s Ice Shell Dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-536, https://doi.org/10.5194/egusphere-egu26-536, 2026.

EGU26-538 | ECS | Orals | PS2.6

Geodynamics of the High Pressure Ice Layer on Ganymede 

Nora van den Heuvel, Ana-Catalina Plesa, Hauke Hussmann, and Christophe Sotin

Jupiter’s moon Ganymede, the largest moon in the Solar System, is the main focus of the JUICE mission, which will observe its surface and measure its interior with unprecedented detail (Van Hoolst et al., 2024). In contrast with smaller moons such as Europa or Enceladus where an ocean is in contact with the silicate interior, Ganymede contains a high pressure (HP) ice layer between its ocean and the rocky core. Thus, on Ganymede, the dynamics in the high pressure ice layer control the exchange of heat and chemical species between the ocean and rocky interior.

 

The thickness of the HP ice layer is not well constrained, and interior structure models suggest thicknesses around 400 km, with values as low as 100 km (Kalousova et al., 2018) and as high as 700 km (Vance et al., 2018). Depending on the thickness of this layer, various polymorphs of HP ice might appear (Hussmann et al., 2015), such as ice V and ice VI, and for a sufficiently cold ocean also ice III (Journaux et al., 2020). Here we focus on ice V and ice VI, as they might exhibit different viscosities that in turn can substantially affect the convective behavior of the HP ice layer. Rheological experiments of ice V and ice VI are rare, but existing studies (Sotin & Poirier, 1987) indicate that ice V can be harder to deform than ice VI, and the viscosity ratio can reach up to three orders of magnitude.

 

We investigate the dynamics of Ganymede’s HP ice layer using the geodynamical code GAIA (Hüttig et al., 2013). Our models use the viscosity formulation of Kalousová et al. (2018) that has been derived from rheological experiments (Sotin et al., 1985; Durham et al., 1996). We test models where the HP ice layer of Ganymede is subdivided into ice V and ice VI layers. Our models vary the reference viscosity of the ice VI layer between 1015 and 1018 Pa s and apply a viscosity contrast between the ice V and ice VI layers of up to 1000. Similar to Choblet et al. (2017), we limit the temperature to the melting temperature of the HP ice layers and compute the amount of melt produced throughout the evolution. Our models consider a decaying heat flow boundary condition at the ice-rock boundary using values from Choblet et al. (2017), and assuming that the heat flow exponentially decreases from 40, 20 or 10 mW/m2 at 4.5 Gyr ago to a present-day value of 5 mW/m2.

 

Our models show that the ice shell dynamics substantially change with the increase of viscosity contrast between ice V and ice VI, leading eventually to a two layered convection structure. Heat and material transport from the ice-rock interface to the ocean occurs in pulses, when convective plumes can penetrate through the upper, high-viscosity ice V layer. Future models will include the effects of tidal heating and track the redistribution of impurities, i.e., salts, through the high pressure ice layers of Ganymede.

How to cite: van den Heuvel, N., Plesa, A.-C., Hussmann, H., and Sotin, C.: Geodynamics of the High Pressure Ice Layer on Ganymede, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-538, https://doi.org/10.5194/egusphere-egu26-538, 2026.

EGU26-2724 * | Orals | PS2.6 | Highlight

The Mission to Enceladus – The ESA L4 mission 

Jörn Helbert, Martin Haag, Tara-Maria Bründl, Bjorn Ordoubadian, Sven Wittig, and Martin Linder and the The L4 Expert Committee and the L4 Payload Working Group

The ESA Voyage 2050 Senior Committee recommended a mission to the “Moons of the Giant Planets” as ESA’s fourth Large-class mission (L4), building on the legacy of Cassini-Huygens and JUICE. ESA’s leadership in planetary science is reaffirmed through this bold initiative to explore ocean worlds and search for biosignatures.

Following this recommendation, ESA convened an Expert Committee to define the mission’s scope. Enceladus emerged as the prime target due to its active plumes and potential for in-situ ocean sampling. Cassini’s 2005 flybys revealed water vapour jets and ice particles erupting from Enceladus’ south pole, with magnetometer data confirming subsurface activity. Surface temperatures around the “tiger stripes” reached −163°C, indicating geological heat sources and active cryovolcanism.

Enceladus meets all three criteria for habitability: liquid water, energy, and essential chemical elements. ESA’s L4 mission will advance this legacy by deploying both an orbiter and a lander—marking the first landing attempt on Enceladus. The lander will analyse icy particles precipitating from the subsurface ocean, potentially rich in salts, organics, and biosignatures.

Since March 2025, ESA’s study team, in collaboration with the Payload Working Group and Expert Committee, has been refining science requirements and identifying enabling technologies. This mission will push European capabilities in in-orbit assembly, extreme environment operations, landing systems, and novel instrumentation—reinforcing ESA’s role as a global leader in space exploration and innovation.

How to cite: Helbert, J., Haag, M., Bründl, T.-M., Ordoubadian, B., Wittig, S., and Linder, M. and the The L4 Expert Committee and the L4 Payload Working Group: The Mission to Enceladus – The ESA L4 mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2724, https://doi.org/10.5194/egusphere-egu26-2724, 2026.

EGU26-3442 | ECS | Posters on site | PS2.6

Onset of Convection affected by Internal Heating - Implications for Europa and Enceladus 

Henry W. Sitte, Teresa Wong, Claudia Stein, and Ulrich Hansen

Europa and Enceladus present two bodies in our Solar System that, besides Earth, contain liquid water and therefore the chance of extraterrestrial life. Regarding the state and evolution of their H2O-layer there are still many open questions. One important mechanism is the heat transport through the outer solid ice shell. It is still unclear whether the ice shells are in a conductive state or if convection takes place. One significant parameter determining if its possible that convection can set in is the ice shell thickness which is unknown for both icy moons. Since both celestial bodies are in the vicinity of enormous planets, namely Jupiter and Saturn, they are subjected to significant tidal forces. These forces can result in additional heating of the ice shell. Due to this further energy source convection might be possible for ice shell thicknesses smaller than predicted by Rayleigh-Bénard convection.
We numerically investigate how an additional uniform internal heating affects the point for the onset of convection in a two-dimensional Cartesian system that is also heated from below. The point for the onset of convection is characterized by the critical Rayleigh number that describes the strength of convection. With an increasing internal heat production rate, the critical Rayleigh number decreases, meaning that less force is required to initiate convection compared to a purely basally heated system. Furthermore, we use these results to derive corresponding minimum ice shell thicknesses. Depending on the viscosity of the ice, we find values between 8 km and 83 km for a system without internal heating that are reduced to 1.5 km to 15 km for the largest investigated heating rate for Europa. For Enceladus, our results yield thicknesses of 22 km to 223 km (no heating) down to 3 km to 30 km (largest heating). Comparing these values to actual estimations of the ice shell thickness for the moons exhibit a realistic chance for Europa’s ice shell to convect but only a small likelihood for Enceladus’ ice shell.

How to cite: Sitte, H. W., Wong, T., Stein, C., and Hansen, U.: Onset of Convection affected by Internal Heating - Implications for Europa and Enceladus, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3442, https://doi.org/10.5194/egusphere-egu26-3442, 2026.

EGU26-3549 | ECS | Posters on site | PS2.6

Protonation-induced chemical transformations of complex organics in mass spectrometry: implications for the exploration of icy moons 

Lucía Hortal Sánchez, Maryse Napoleoni, Ernesto Brunet, Fabian Klenner, Thomas R. O'Sullivan, Mirandah Ackley, Gregoire Danger, Bernd Abel, Nozair Khawaja, and Frank Postberg

Impact ionisation mass spectrometers, such as the Cosmic Dust Analyser (CDA) onboard Cassini and the SUrface Dust Analyzer (SUDA) onboard Europa Clipper, are key instruments to investigate the composition of icy ocean moons1. They are capable of detecting organics in ice grains ejected from cryovolcanic processes (e.g. Enceladus’ plume) and micrometeoritic bombardment of the icy surface. Laboratory analogue experiments that replicate ice grain impact ionisation mass spectra are crucial in order to reliably identify chemical features of organics in spacecraft data. The laser-induced liquid beam ion desorption (LILBID) technique allows the accurate simulation of impact ionisation mass spectra at a range of impact velocities, by desorbing ionic and neutral molecules and fragments from a μm-sized liquid beam containing water and dissolved analytes2. This work investigates amygdalin (C20H27NO11) and its mass spectral fingerprint with LILBID, aiming to assist in the analysis of organic molecules with impact ionisation mass spectrometry. Upon measurement, amygdalin undergoes protonation-induced chemical transformations (PICTs), enabled by the high laser energy input and proton-rich environment created upon disintegration of the water matrix. The observed reactivity is a distinct phenomenon that can be set apart from other well-characterised processes that analytes can be subject to upon measurement with LILBID and impact ionisation mass spectrometry (e.g. fragmentation). PICTs observed in amygdalin feature its initial nitrile group as well as other functional groups obtained after the first transformation (e.g. carboxylic acid), resulting in multiple reactions products identified by their characteristic molecular ions. Complementary measurements with nuclear magnetic resonance spectroscopy confirmed that reactivity does not occur in solution prior to desorption, and must therefore occur under LILBID measurement. In principle, functional groups similar to nitrile (e.g., amide or ketone) in other compounds could also be subject to PICTs. PICTs may also occur with spaceborne impact ionisation, potentially complicating the identification of organics contained in ice grains. This work builds towards a better understanding of PICTs and their effect(s) on the detection of organic compounds using impact ionisation mass spectrometry, and has key implications for the interpretation of Cassini’s CDA data and for investigations of the composition of icy ocean moons with upcoming space missions (e.g. Europa Clipper or ESA’s large-class mission to Enceladus).

[1] S. Kempf et al., Space Sci. Rev. 221, 10 (2025)

[2] F. Klenner et al., Rapid Comm. Mass Spectrometry 33 (22), 1751–1760 (2019)

How to cite: Hortal Sánchez, L., Napoleoni, M., Brunet, E., Klenner, F., O'Sullivan, T. R., Ackley, M., Danger, G., Abel, B., Khawaja, N., and Postberg, F.: Protonation-induced chemical transformations of complex organics in mass spectrometry: implications for the exploration of icy moons, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3549, https://doi.org/10.5194/egusphere-egu26-3549, 2026.

EGU26-3571 | ECS | Posters on site | PS2.6

The modulation effect of ice thickness variations on convection in icy ocean worlds 

Wanying Kang and Shuang Wang

It has been long puzzling whether the ice thickness variations observed on Enceladus can be sustained solely by a polar-amplified bottom heating. The key to this question is to understand how the upward heat transport by convective plumes would be interfered by the temperature and salinity variations beneath the ice due to the ice thickness variations, which however, has yet to be explored. Here, we find that the horizontal temperature variation induced by the ice topography can easily be orders of magnitude greater than the vertical temperature variation induced by bottom heating using scaling analysis. Due to the dominance of horizontal temperature gradient, convective plumes are completely shut off by a stratified layer under the thin ice formed out of baroclinic adjustment, largely slowing down the vertical tracer transport. The stratified layer will also deflect almost all of the core-generated heating toward the regions with thicker ice shell, destroying the ice thickness gradient. These results allow us to put an upper bound on the core-generated heating on Enceladus, which is crucial for the estimate of habitability. Scaling laws for the bottom heat flux to penetrate the stratification is derived and examined. This scaling can be used to constrain the maximum ice thickness variations induced by heterogeneous bottom heating on icy satellites in general, which can be used to differentiate icy satellites that generate the majority of heat in the ice shell from those that generate the majority of heat in the silicate core.

How to cite: Kang, W. and Wang, S.: The modulation effect of ice thickness variations on convection in icy ocean worlds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3571, https://doi.org/10.5194/egusphere-egu26-3571, 2026.

EGU26-3594 | Posters on site | PS2.6

Comparative Planetology of Earth and Titan through Analog Research 

Conor Nixon and the Titan Analog Study Team

Saturn’s moon Titan exhibits remarkable parallels with Earth in a range of geophysical and geological processes not found elsewhere in the solar system at the present day. These include a nitrogen-rich atmosphere with a condensable gas - methane replacing water - leading to an active meteorological cycle with rainfall and surface expressions including rivers, lakes and seas, and the dissolution of karstic terrain. Other phenomena such as craters, dunes, and tectonic features are found elsewhere - e.g. on Mars and Venus - but their continuing alteration by pluvial, fluvial, and lacustrine processes can be studied only on Earth and Titan. Titan also hosts a subsurface liquid water ocean with similarities to the Earth as well as ocean worlds such as Europa and Enceladus. Here, we describe the geophysical and geological parallels between Earth and Titan and suggest yet-underexploited possibilities for field analog research to gain new knowledge about these processes. To date, Titan’s much colder temperature and distinct atmospheric and surface compositions have led to a skepticism with regard to usefulness of terrestrial analogs. Our conclusion, however, is that a much larger range of useful field analog work is possible and this work will substantially enhance our knowledge of both worlds. Such investigation will supplement the existing sparse data for Titan returned by space missions, will greatly enhance our understanding of such datasets, and will help to provide science impetus and goals for future missions.

How to cite: Nixon, C. and the Titan Analog Study Team: Comparative Planetology of Earth and Titan through Analog Research, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3594, https://doi.org/10.5194/egusphere-egu26-3594, 2026.

Assembly and test of the DraGMet Flight Model (FM) hardware for Dragonfly’s July 2028 launch has begun. The Flight Model seismometer was delivered from JAXA in October 2025 and has been integrated with the APL winch assembly and has undergone vibration and other tests. The flight lot of wind sensors have been performance-tested in the Titan Pressure Environment Chamber at APL, and the best-performing units selected as FMs and spares. An opportunity also arose to test the wind sensor design in a heavy gas (1,1,1,2-tetrafluoroethane, R-134a) atmosphere in the Transonic Dynamics Tunnel (TDT) at NASA Langley Research Center during aerodynamic tests on the Dragonfly vehicle. I will review these and other progress highlights of DraGMet which comprises 12 different sensor types with a common DPU to explore the atmosphere, surface and interior of Titan less than 9 years from now.

How to cite: Lorenz, R.: Development of Geophysics and Meteorology Sensors for Titan : Update on Dragonfly’s DraGMet package, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5947, https://doi.org/10.5194/egusphere-egu26-5947, 2026.

EGU26-6551 | ECS | Posters on site | PS2.6

Elastic Plastic Flexure on Icy Moons: Implications for heat flux 

Adrien Broquet

Investigations of ice-shell flexure, as observed from stereo-derived topographic profiles, have been commonly used to provide information on the interior structure and evolution of icy moons (e.g., Nimmo et al., 2002, Peterson et al., 2015). The most commonly used approach is to fit the observed flexure to an elastic plate model to infer the local elastic thickness of the body’s ice shell at the time of deformation. The widespread use of this approach lies in its quick analytical expression, allowing to test various parameters at multiple locations (e.g., Turcotte & Schubert, 2002). However, it remains unclear whether elastic plate models can be used to reliably predict the flexure of an elastic-plastic ice shell.

For geologic interpretations, the elastic thickness parameter can be converted to a heat flux using several approaches. First, by setting the bending moment of the elastic plate equal to the bending moment of a more realistic plate with a rheology that considers fracturing and viscous flow (e.g., McNutt, 1984). One critical issue during this approach is related to the selection of the input curvature of the plate, which affects the calculation of the bending moment. Alternative approaches have assumed the base of the elastic lithosphere to be defined by a rheology-dependent isotherm in combination with a specific Deborah number (e.g., Nimmo et al., 2002). However, it remains unclear what Deborah number should be assumed when the plate is elasto-plastic and whether both the equal-bending moment and the Deborah number approaches lead to similar results.

In this work, we follow the framework developed in Mueller & Phillips (1995), to test the applicability of elastic plate models to icy satellites. We show that the maximum curvature of the synthetic elastic flexural profile should be used when relating elastic thickness to heat flux and discuss that purely elastic models predict unrealistic oscillations near and in the flexural bulge region. Finally, we reveal that previous work that used the Deborah number approach substantially overestimated the heat flux of Ganymede (Nimmo et al., 2002) and Ariel (Peterson et al., 2015), with implications for the geologic history of these icy worlds.

 

McNutt, M. K. (1984). Lithospheric flexure and thermal anomalies. J. Geophys. Res.: Solid Earth, 89. doi: 10.1029/jb089ib13p11180.

Mueller, S. and R. J. Phillips (1995). On the reliability of lithospheric constraints derived from models of outer-rise flexure. Geophys. J. Int., 123. doi:10.1111/j.1365- 246x.1995.tb06896.x

Nimmo, F.,  Pappalardo, R.T., & Giese, B. (2002). Effective elastic thickness and heat flux estimates on Ganymede, Geophys. Res. Lett., 29(7), doi:10.1029/2001GL013976.

Peterson, G., F. Nimmo, and P. M. Schenk (2015). Elastic thickness and heat flux estimates for the Uranian satellite Ariel, Icarus 250, doi: 10.1016/j.icarus.2014.11.007.

Turcotte, D. L. and G. Schubert (2002). Geodynamics. Cambridge University Press. doi: 10.1017/cbo9780511807442.

How to cite: Broquet, A.: Elastic Plastic Flexure on Icy Moons: Implications for heat flux, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6551, https://doi.org/10.5194/egusphere-egu26-6551, 2026.

EGU26-7016 | Orals | PS2.6

Layered bubble-rich structures on icy worlds: experiments with large volumes of low-salinity water in near-vacuum environment. 

Vojtěch Patočka, Petr Brož, Kristian Chan, Priyanka Biju Sindhu, Mark Fox-Powell, Matthew Sylvest, Zoe Emerland, and Manish Patel

While the geysers on Enceladus are a spectacular example of explosive cryovolcanic eruptions, active cryovolcanic effusions have not been observed in the Solar System. Signs of former cryoeffusions are only indirect, including smooth terrains with morphological resemblance to volcanic flows on Earth (Fagents, 2003; Lesage et al., 2020), thermal anomalies (Abramov and Spencer, 2009), or excess atmospheric volatiles (Quick et al., 2017). As a result, our ability to investigate the processes involved in their emplacement remains limited.

Several theoretical models have been proposed to explain and describe the origin and behavior of effusive cryovolcanism, that is, the ascent and release of subsurface water onto the surface (Allison and Clifford, 1987; Quick et al., 2017; Lesage et al., 2020). In general, water exposed to the cold, near-vacuum surface environments of icy bodies is expected to freeze with a porous skin (Bargery et al., 2010). A vast uncertainty remains, however, regarding how long it takes, how much material is lost due to vaporization and sublimation, and how porous the resulting ice is (Morrison et al., 2023; Brož et al., 2025).

In the presented work (Patočka et al., 2026), we expose 40 kg of low-salinity water in a specialist chamber at The Open University, UK, and show that freezing under near-vacuum conditions is a complex, dynamic process during which vapor puffs through the growing ice sheets, building previously unobserved ice structures. Millimeter-thin, sheet-like ice layers form, separated by centimeter-thick, large-aspect-ratio pockets of vapor. The overall height of this layered, bubble-rich ice is controlled by a balance between its weight and the equilibrium vapor pressure. In the laboratory, the height reaches approximately ten centimeters, which could plausibly extend to tens of meters in the low-gravity environments of icy bodies. The high porosity of such ice has significant implications for the interpretation of remote sensing observations, and its fragile character makes terrains created by effusive cryovolcanism hazardous for spacecraft landing. 

This work was funded by the Czech Grant Agency grant No. 25- 15473S. VP has been supported by the Charles University Research Centre program No.~UNCE/24/SCI/005. MRP acknowledges support from the UK Space Agency/STFC through grants UKRI2545, ST/X006549/1, ST/Y005929/1, ST/Y000234/1 and ST/X001180/1.

References:

Abramov, O., Spencer, J.R., 2009, doi:10.1016/j.icarus.2008.07.016.
Allison, M., Clifford, S., 1987, doi.org/10.1029/JB092iB08p07865
Bargery, A.S., Lane, S.J., Barrett, A., Wilson, L., Gilbert, J.S., 2010, doi:10.1016/j.icarus.2010.06.019.
Brož, P., Patočka, V., Butcher, F., Sylvest, M., Patel, M., 2025, doi:10.1016/j.epsl.2025.119531.
Fagents, S.A., 2003, doi:10.1029/2003JE002128.
Lesage, E., Massol, H., Schmidt, F., 2020, doi:10.1016/j.icarus.2019.07.003.
Morrison, A.A., Whittington, A.G., Mitchell, K.L., 2023, doi:10.1029/2022JE007383.
Patočka, V., Brož, P., Chan, K., Sindhu, P., Fox-Powell, M., Sylvest, M., Emerland, Z., Patel, M., 2026, submitted

How to cite: Patočka, V., Brož, P., Chan, K., Sindhu, P. B., Fox-Powell, M., Sylvest, M., Emerland, Z., and Patel, M.: Layered bubble-rich structures on icy worlds: experiments with large volumes of low-salinity water in near-vacuum environment., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7016, https://doi.org/10.5194/egusphere-egu26-7016, 2026.

EGU26-7511 | Orals | PS2.6

Indication of an unusual atmospheric loss event at Titan  

howard smith and Robert Johnson

Observations from the Cassini mission revealed cryogenic water plumes from the small moon Enceladus are the dominant source of heavy material in Saturn’s magnetosphere. This fascinating insight indicates that a relatively small body dominates the entire giant planet magnetosphere. However, no evidence of magnetospheric impact was observed from Titan, despite this moon being much large with a very dense, unprotected (nitrogen dominated) atmosphere.  Interestingly, more recent data analysis of the entire Cassini dataset indicates Titan can experience previously unknown brief active periods. In particular, global magnetospheric energetic ion composition modifications were observed originating from an abrupt increase in Titan atmospheric loss. We characterize this event and discuss the possible causes as: (1) a methane cycle interruption; (2) an impact event; (3) enhanced surface activity; and/or (4) transiently enhanced solar wind exposure. Our results indicate that such activity can impact the entire magnetosphere and opens up the possibility for similar atmospheric loss events on other bodies.

How to cite: smith, H. and Johnson, R.: Indication of an unusual atmospheric loss event at Titan , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7511, https://doi.org/10.5194/egusphere-egu26-7511, 2026.

EGU26-7582 | ECS | Posters on site | PS2.6

Horizontal Convection in Icy Satellite Oceans with Melting and Freezing  

Hamish Hay, David Rees Jones, Eric Hester, and Daphné Lemasquerier

Thermal buoyancy is a primary driver of icy-satellite ocean dynamics, caused by mantle heating at the seafloor and cooling at the ice–ocean interface. A significant driver of mantle heating is dissipation by cyclic tidal deformation. When this buoyancy forcing is spatially uniform, laboratory and numerical experiments have shown that it can create overturning circulation, melting and freezing of the overlying ice, and alternating east–west jets of rapid circulation. Tidal dissipation, however, naturally varies in space, causing differential heating of the ocean bottom. These temperature variations will drive horizontal convection, a large-scale overturning circulation with a zonal structure. Here, we investigate the mechanics of this horizontal convection, its interaction with Rayleigh-Bénard (vertical) convection, and dynamic feedback with ice-shell thickness, melting, and freezing. 

We perform non-rotating simulations of convection in a 2D Cartesian geometry with a mobile ice–ocean interface using the pseudo-spectral code, Dedalus. A sinusoidal temperature profile is imposed on the bottom of the ocean as well as a vertical (average) temperature difference. The relative amplitude of horizontal to Rayleigh-Bénard convection is varied by changing the ratio of the vertical to horizontal temperature differences, as well as the aspect ratio of the domain. The phase change between pure water and ice is captured using the phase field method. We perform sensitivity tests to determine the optimum phase field parameters that best approximate stagnation-point flow solutions in the vicinity of the ice–ocean interface. These optimum parameters vary as a function of vertical Rayleigh number. We then investigate the competition between Rayleigh-Bénard and horizontal convection without phase change, before including melting and freezing to study the dynamic feedback of ice topology on this competition. Finally, we seek to place our simulations in the context of icy-satellite oceans by determining scaling relationships between the horizontal Rayleigh and Nusselt numbers.  

How to cite: Hay, H., Rees Jones, D., Hester, E., and Lemasquerier, D.: Horizontal Convection in Icy Satellite Oceans with Melting and Freezing , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7582, https://doi.org/10.5194/egusphere-egu26-7582, 2026.

EGU26-7604 | ECS | Posters on site | PS2.6

Ice–ocean interactions as a driver of basal ice roughness and ice shell evolution on Europa 

Christian Maas, Antoniette Greta Grima, and Ulrich Hansen

Europa’s ice shell is thought to overlie a global liquid water ocean, with exchange of heat and momentum across the ice–ocean boundary playing a fundamental role in shaping the shell’s structure and dynamics. Previous studies have shown that heterogeneous ocean circulation and tidal heating can imprint spatially variable heat flux and thus melting and freezing at the ice–ocean interface. However, how the ocean’s thermal state and convective vigour influence the morphology of the ice–ocean interface itself remains poorly understood. Here, we investigate coupled ice–ocean dynamics relevant to Europa in a two-dimensional annulus geometry, with the phase transition between the liquid water ocean and the solid ice layer treated self-consistently through a phase-field approach. Spatially variable temperature anomalies are imposed following Lemasquerier et al. (2023), allowing us to explore the effects of heterogeneous tidal heating under different ocean thermal regimes. We find that colder oceans lead to thicker ice shells and systematically rougher ice–ocean interfaces, characterised by enhanced basal ice topography, which may lead to stronger lateral variability in melting and freezing rates. We also note that as the temperature anomaly between the poles and equator increases, heat transport becomes strongly asymmetric. This results in hemispheric-scale contrasts in ice thickness and the formation of two distinct ice hemispheres separated by a global ocean band confined to low latitudes. These conditions promote the development and persistence of basal roughness on spatial scales comparable to large-scale ice shell heterogeneity. Basal ice roughness and associated thickness variations are expected to strongly influence ice shell dynamics by driving lateral ice flow, promoting ice fabric development, and enhancing lateral stress focusing. On Europa, such mechanically heterogeneous ice shells may play a key role in localising deformation, modulating fracture patterns, and controlling pathways for ocean–ice exchange. Our results highlight the ice–ocean interface morphology as a critical, yet often overlooked, outcome of ice–ocean coupling, with important implications for the evolution and dynamics of Europa’s ice shell.

How to cite: Maas, C., Grima, A. G., and Hansen, U.: Ice–ocean interactions as a driver of basal ice roughness and ice shell evolution on Europa, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7604, https://doi.org/10.5194/egusphere-egu26-7604, 2026.

EGU26-7633 | Orals | PS2.6

Self-consistent modelling of Titan's upper atmosphere: energy balance, photochemistry, and Jeans escape 

Sudeshna Boro Saikia, Jonathan Tennyson, Shuchen Ji, Nils-Martin Robeling, Ivan Stanković, Gwenaëlle Van Looveren, Simon Schleich, Colin Johnstone, Kristina Kislyakova, and Manuel Güdel

Titan’s atmosphere provides a unique laboratory to study how photochemistry, photoionisation, radiative and escape processes shape the atmospheric properties of a nitrogen-rich atmosphere very different from Earth’s. We present a new extension of the 1D first principles upper atmospheric code Kompot, and benchmark it against Titan’s thermosphere. The code self-consistently calculates the thermal and chemical structure of Titan’s upper atmosphere by solving the coupled hydrodynamic, photochemical kinetic, and energy balance equations. The energy balance equation is primarily set by heating due to stellar X-ray and ultraviolet (XUV) and infrared radiation, chemical heating, radiative cooling by methane(CH4) and hydrogen cyanide (HCN), and thermal conduction. We calculate XUV heating from first principles and do not use any efficiency factor. Our model results are in good agreement with Cassini-Huygens and ALMA observations of Titan. The simulated abundances of the key molecular species, including CH4, also show strong agreement with Cassini-Huygens results. Molecular hydrogen has the strongest thermal Jeans escape in our model, where as the thermal escape of CH4 is negligible. Our results suggest that present-day Titan’s CH4 abundance at the upper thermosphere can be explained by a self-consistent model without invoking strong atmospheric escape.

How to cite: Boro Saikia, S., Tennyson, J., Ji, S., Robeling, N.-M., Stanković, I., Van Looveren, G., Schleich, S., Johnstone, C., Kislyakova, K., and Güdel, M.: Self-consistent modelling of Titan's upper atmosphere: energy balance, photochemistry, and Jeans escape, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7633, https://doi.org/10.5194/egusphere-egu26-7633, 2026.

EGU26-7799 | Posters on site | PS2.6

Contributions of saline meltwater to ice flow and its remote sensing signatures 

Cassandra Seltzer, Hatsuki Yamauchi, Caitlin Huntsman, Christine McCarthy, Andrew Cross, and Benjamin Hills

Icy moon interiors and terrestrial glacier environments often contain a degree of saltwater melt. This liquid phase can modify the flow of ice, creating preferred directions for deformation through a melt preferred orientation (MPO) that may form in response to stress. Ice crystals adjust on the microscale to drive flow, imparting a crystallographic orientation fabric (COF) that can also be measured to infer the subsurface stress and strain conditions. We show results from laboratory experiments on compressive flow, characterizing the response of both ice crystals and saltwater melt as they together define the geophysical properties of multiphase, partially melted ice. We observe conclusively that an MPO forms parallel to the compressive stress direction, enhancing and possibly tracking material flow, and note that the extent of solid material deformation may decrease with increasing melt fraction. Finally, we combine evolving COF and MPO to define potential radar sounding returns as indicators of subsurface flow, finding that MPO imparts distinct signatures that may be useful in decoding the stress and strain state of icy settings from remote sensing observations. 

How to cite: Seltzer, C., Yamauchi, H., Huntsman, C., McCarthy, C., Cross, A., and Hills, B.: Contributions of saline meltwater to ice flow and its remote sensing signatures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7799, https://doi.org/10.5194/egusphere-egu26-7799, 2026.

EGU26-10209 | Posters on site | PS2.6

Toward an appropriate flow law to model icy moons tidal and convective deformation 

Maurine Montagnat, Maria-Gema Llorens, Soroush Motahari, Ana-Catalina Plesa, Christophe Sotin, and Gabriel Tobie

Flow laws describe how ice deforms as a function of a number of parameters, such as strain, stress, grain-size, temperature, anisotropy or pressure. They are critical to describe the flow of terrestrial glaciers and the tidal and convective deformation taking place in icy moons. 
However, whereas Glen’s law is used in the cryosphere science community, the so-called Goldsby and Kohlstedt flow law is used in the icy moon community. 
How different are these two types of law? What are their limitations and domain of applicability? 
In this work, we first remind the origin and the assumptions behind these two types of law. We then get back to the physics of the deformation processes of concern, in the case of tidal forcing (very low cumulated strain) or convective deformation (very low stresses) to highlight the limits of applicability of the laws. 
Using existing laboratory experiments and field measurements we investigate and help inferring the best law to use and provide some illustrations of the impact on the convective response.

How to cite: Montagnat, M., Llorens, M.-G., Motahari, S., Plesa, A.-C., Sotin, C., and Tobie, G.: Toward an appropriate flow law to model icy moons tidal and convective deformation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10209, https://doi.org/10.5194/egusphere-egu26-10209, 2026.

EGU26-11450 | Orals | PS2.6

Identification of Molecular Biosignatures in Antarctic Ices: Implications for Icy Moons Exploration 

Maryse Napoleoni, Lucía Hortal Sánchez, Pablo L. Finkel, Daniel Carrizo, Laura Sánchez-García, David Burr, Florence Hofmann, Mercedes Moreno Paz, Nozair Khawaja, Victor Parro, and Frank Postberg

Enceladus and Europa are key targets for planetary exploration due to their subsurface water oceans, making them some of the most habitable places in the solar system. Onboard the Europa Clipper spacecraft, the SUrface Dust Analyzer (SUDA [1]) will provide the chemical composition of ice grains ejected by plumes and/or micrometeorite bombardment of the surface. As shown by laboratory experiments [e.g., 2,3], molecular biosignatures can be detected by SUDA or an alternative advanced mass spectrometer on an Enceladus mission [4]. Lipids in particular can provide characteristic spectral fingerprints and are considered universal biomarkers of life [5] owing to their effective membrane-forming properties even under geochemically hostile conditions and their ubiquity in all known forms of life.

The performance and calibration of SUDA-type instruments strongly relies on analogue experiments using Laser Induced Liquid Beam Ion Desorption (LILBID) - a well-established method allowing the simulation of ice grains’ impact ionization mass spectra. Many LILBID spectra have already been recorded to complement an expanding reference database [6] for e.g., Europa Clipper.Environmental samples allow for a more realistic assessment of the detection capabilities of spaceborne instruments (as compared to experiments with prepared synthetic samples of well-defined compositions). Specifically, natural ice analogues from polar locations offer some of the most realistic representations of icy moons. However, polar samples have never before been analyzed with LILBID.

Here we present the first analysis of natural ice analogues with LILBID combined with a detailed characterization of lipid biomarkers. With support from the Instituto Antártico Uruguayo, ice samples were collected from key locations in the Collins (a.k.a. Bellingshausen) glacier on King George Island, Antarctica, where several environmental conditions (including intense UV radiation, saline aerosols, low temperature) are analogous to specific processes on ocean worlds.

LILBID analysis, providing SUDA-type analogue mass spectra, were combined to data obtained from Gas Chromatography linked to Mass Spectrometry (GC-MS), Raman and IR spectroscopy. Results on icy samples containing pink microalgae revealed key fingerprints of lipids adapted to cold temperatures, and highlight a novel assessment of the detectability of lipid biomarkers from icy moon analogues with spaceborne instrumentation.

[1] S. Kempf et al., Space Sci. Rev. 221, 10 (2025); [2] M. Dannenmann et al. Astrobiology 23(1):60–75 (2023); [3] F. Klenner et al., Science Advances, 10(12), eadl0849 (2024); [4] O. Mousis et al., The Planetary Science Journal, 3(12), 268 (2022); [5] C.D. Georgiou & D.W. Deamer. Astrobiology 14(6):541–549 2014); [6] F. Klenner et al., Earth Space Sci., 9, e2022EA002313 (2022)

How to cite: Napoleoni, M., Hortal Sánchez, L., Finkel, P. L., Carrizo, D., Sánchez-García, L., Burr, D., Hofmann, F., Moreno Paz, M., Khawaja, N., Parro, V., and Postberg, F.: Identification of Molecular Biosignatures in Antarctic Ices: Implications for Icy Moons Exploration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11450, https://doi.org/10.5194/egusphere-egu26-11450, 2026.

EGU26-11571 | ECS | Orals | PS2.6

Turbulent zonal jets interacting with isolated topography: an experimental study 

Daphné Lemasquerier, Cy David, Rémy Monville, and Jonathan Aurnou

Zonal jets are coherent east-west winds or currents observed –or expected to emerge– in many planetary fluid layers, from the Earth’s oceans and atmosphere, to the atmospheres of gas giants, the subsurface oceans of icy moons and the liquid metallic cores of telluric planets. In many of these systems, zonal jets interact with a solid boundary with topography: the bathymetry in Earth’s oceans is known to influence the dynamics of the Antarctic Circumpolar Current, flows in liquid cores interact with the topography at the Core-Mantle boundary, and icy moon oceans are in direct contact with a global ice crust of spatially varying thickness.

In this talk, I will present laboratory experiments to study the interaction between self-sustained turbulent zonal jets and an isolated topography. We use the Coreaboloid device at UCLA (Lonner et al., 2022, doi:10.1029/2022JE007356) to robustly produce turbulent zonal jets. The setup is a 75cm-diameter water tank rotating at speeds up to 72 revolutions per minute. The deflection of the free surface due to the fast rotation provides a strong topographic β-effect. The flow is forced by thermal convection, driven by starting the experiment with hot water, and cooling the inner cylinder with a block of ice. To simulate a localised topography, we attach acrylic disks of different radii and heights on the bottom plate. We visualise the flow using 1) a thermal infrared camera to image the temperature field at the free surface 2) particle image velocimetry (PIV) on a horizontal laser plane and 3) ultrasonic doppler velocimetry (UDV) along three chords. We find that stationary Rossby waves develop downstream of the topography in prograde jets and influence the amplitude, number, and position of the zonal jets. The observed zonal wavelength of stationary lee Rossby waves agrees with theoretical predictions for plane Rossby waves, provided that the feedback of the zonal flow amplitude and curvature is taken into account. Remarkably, the topography leaves a visible imprint on the flow even for heights as small as h=3 mm, corresponding to just 1.2% of the total fluid depth H. For larger topography (h/H=5.9% to 17.5%), upstream blocking is observed, and a cyclonic circulation forms above the topography.

How to cite: Lemasquerier, D., David, C., Monville, R., and Aurnou, J.: Turbulent zonal jets interacting with isolated topography: an experimental study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11571, https://doi.org/10.5194/egusphere-egu26-11571, 2026.

EGU26-11843 | Posters on site | PS2.6

Radar Observations of Titan's Hydrocarbon Seas and Lakes: Refining Liquid Composition and Seafloor Properties 

Marco Mastrogiuseppe, Giada Vallecoccia, Maria Carmela Raguso, and Daniele Durante

Introduction: The Cassini RADAR altimeter enabled the first direct bathymetric measurements of an extraterrestrial sea by sounding liquid hydrocarbon bodies on Titan. These observations revealed that Titan’s seas are remarkably transparent at Ku-band frequencies with depths that can reach several hundreds of meters. Measurements of the electromagnetic properties of the liquids further indicated a methane-dominated composition, with minor contributions from ethane and nitrogen [1]. Together, these results provided robust quantitative constraints on Titan’s hydrocarbon inventory and on the dielectric properties of its surface liquids.

More recently, re-analyses of Cassini Synthetic Aperture Radar (SAR) observations using multi-angular scattering models have independently characterized the dielectric and roughness properties of solid terrains in Titan’s north polar region. This study revealed systematic differences between radar-bright and radar-dark surface units, providing new insights into compositional and morphological heterogeneity across Titan’s polar regions [2].

Seafloor–Surface Scattering Comparison and Liquid Loss Tangent Refinement: In this work, we directly compare the radar backscattering properties of Titan’s seafloors, inferred from combined Cassini RADAR altimetry and SAR observations, with those of exposed solid surfaces characterized through multi-angular scattering analyses. This combined approach enables improved isolation of attenuation effects associated with the overlying liquid column, allowing refinement estimates of the liquid loss tangent, and improved constraints on the dielectric properties of the underlying seafloor. Particular emphasis is placed on Ligeia Mare, for which we derive an independent estimate of the liquid loss tangent using SAR data, yielding to a more accurate electromagnetic characterization of Titan’s second-largest hydrocarbon sea.

Figure 1. Synthetic Aperture Radar (SAR) mosaic of Titan’s northern polar region showing the distribution and morphology of liquid-filled basins and channels. Yellow lines highlight the major liquid bodies, Figure adapted from [3].

 

Acknowledgements: This work was supported by Italian Space Agency (ASI), contract 2025-4-U.0

References:

[1] Mastrogiuseppe, M., Poggiali, V., Hayes, A., Lorenz, R., Lunine, J., Picardi, G., ... & Zebker, H. (2014). The bathymetry of a Titan sea. Geophysical Research Letters, 41(5), 1432-1437.

[2] M. Mastrogiuseppe et al., "Characterization of Titan’s Northern Polar Terrains From Inversion of Cassini RADAR Data," in IEEE Transactions on Geoscience and Remote Sensing, vol. 64, pp. 1-17, 2026, Art no. 4500117, doi: 10.1109/TGRS.2025.3647365.

[3] Mastrogiuseppe, M., Poggiali, V., Hayes, A.G. et al. Deep and methane-rich lakes on Titan. Nat Astron 3, 535–542 (2019). https://doi.org/10.1038/s41550-019-0714-2

How to cite: Mastrogiuseppe, M., Vallecoccia, G., Raguso, M. C., and Durante, D.: Radar Observations of Titan's Hydrocarbon Seas and Lakes: Refining Liquid Composition and Seafloor Properties, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11843, https://doi.org/10.5194/egusphere-egu26-11843, 2026.

Subsurface oceans hosted by icy bodies in the outer Solar System—such as Europa, Ganymede, Enceladus, Titan, and even dwarf planets like Ceres and Pluto—are prime targets for astrobiological exploration due to their potential to sustain habitable environments. Accordingly, numerous space missions, including JUICE, Europa Clipper, Dragonfly, Dawn, and New Horizons, are designed to investigate the internal structures, thermal states, and chemical environments of these worlds. Recent studies have highlighted the critical role of clathrate hydrates, which exhibit lower thermal conductivity and higher viscosity than water ice, thereby significantly influencing heat transport (convection and conduction), rheological properties, and long-term ocean stability.
Building on the hydrate–ice mixing model (Miller et al., 2025), we aim to systematically incorporate the dynamic integration of clathrate hydrates into a time-dependent thermal evolution framework across a broad parameter space. Our model improvements focus on several key aspects. First, we will consider multiple scenarios for radioactive element abundances, including both long-lived and short-lived radionuclides, and examine how accretion and differentiation time affect internal heating histories. Second, the release and redistribution of methane and other volatile gases are dynamically coupled to core temperature evolution. Third, to extend the model to large icy moons such as Europa, Ganymede, and Titan, we will explicitly include tidal heating and account for high-pressure phases of ice and clathrate hydrates. Fourth, porosity evolution and radius changes are incorporated to explore potential implications for internal structure and surface morphology.
We will first apply the optimized model to Ceres as a benchmark case, exploring how different hydrate–ice mixing states affect its internal structure and the evolution of a potential subsurface ocean. Preliminary expectations suggest that clathrate hydrates may facilitate ocean formation and prolong ocean stability. The refined model will then be applied to Europa, Ganymede, and Titan, where the inclusion of hydrate layers is expected to reduce the energetic requirements for sustaining subsurface oceans, resulting in more physically consistent thermal and structural evolution scenarios.
These results can provide new insights into the chemical and physical controls on the evolution of icy ocean worlds and support the interpretation of forthcoming mission data.

How to cite: zhang, M.: Dynamic Integration of Clathrate Hydrates in the Thermal Evolution of Subsurface Oceans on Icy Moons, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12901, https://doi.org/10.5194/egusphere-egu26-12901, 2026.

Acetylene (C2H2) is the most abundant solid product of methane photochemistry in Titan’s stratosphere. Unlike ethane (C2H6), it does not form a liquid under surface conditions. It should be widespread across Titan’s surface, and yet it hardly, if at all, appears in VIMS spectroscopic data. Where is the acetylene? Both chemical and physical processes are at play on the surface. Preliminary results from a production-loss-transport model of acetylene showing substantial depletion of pure acetylene on the equatorial and mid-latitude regions of Titan are presented. Production is by atmospheric photochemistry and sedimentation in aerosols to the surface. Solid acetylene is metastable and so physical disturbances (see below) can induce cyclization to benzene (C6H6) or polymerization to various forms of polyacetylene (with interesting physical properties).  Reaction with surface HCN (produced by atmospheric chemistry in somewhat lesser amounts) or other nitriles or imines at first glance would be thermally inhibited, but recent calculations of quantum tunneling under Titan conditions suggests acceleration of reaction rates by many orders of magnitude, and so that chemistry is included here. Physical transport is latitudinal, by sublimation/condensation (acetylene is volatile enough to be moved from equator to pole on timescales of 105 years), and from highlands to lowlands by mechanical transport during the intense methane rainfall events observed by Cassini. Aeolian processes, including particle growth (to the sand-sized material in the dunes) and triboelectric charging are included. Static discharge and mechanical disturbance due to aeolian and fluvial processes provide the disturbances to include cyclization or polymerization.   The variation of sunlight through axial precession is relevant on the timescale of sublimation.  Surface gardening by micrometeoroids is unimportant because of the thick atmosphere. Localized processes around lakes and seas, such as dissolution and co-crystal formation, will have a small effect on the overall global budget of acetylene. The predicted abundances and geographic distribution of the acetylene and its products will inform JWST spectroscopic observations and the in-situ investigations by Dragonfly.

Part of this work was performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA.

How to cite: Lunine, J. I.: The Physical and Chemical Life Cycle of Acetylene on Titan’s Surface, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13920, https://doi.org/10.5194/egusphere-egu26-13920, 2026.

We ask what may drive Europa’s putative intermittent plumes. We test whether shallow pockets of liquid water (i.e., sills) freezing within Europa's ice shell can power activity. We build a numerical model that couples heat flow, phase change, and pressure evolution, including the drop in melting temperature under pressure. As a sill freezes, the expansion of ice raises pressure; when a fracture opens, pressure falls and any supercooled liquid crystallizes quickly, producing bursts of solidification, pressure release, and re-pressurization. This cycle can yield sporadic venting and seismic events without a sustained conduit. Pressure-dependent melting shortens the total freezing time at depth and produces rarer but larger events, while elastic flexing of the ice roof reduces the event rate. For reasonable sill sizes and numbers, our model predicts late-stage spikes consistent with sporadic plumes and low-magnitude quakes. These results identify freezing sills as a self-contained engine for Europa’s activity and provide testable signatures for upcoming missions to seek Europaquakes and plumes.

How to cite: Ojha, L.: Europaquakes and Plumes Powered by Freezing-Driven Overpressure, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14210, https://doi.org/10.5194/egusphere-egu26-14210, 2026.

EGU26-14572 | ECS | Orals | PS2.6

Exploring Exogenic Sources of Plume H2 at Enceladus 

Robert W. Grayson and Tom A. Nordheim

Cassini’s exploration of Enceladus’ plume provided tantalizing glimpses into the chemistry of the moon’s interior ocean. The abundance of H2 in the plume, for instance, seems to suggest hydrothermal processes operating within Enceladus’ ocean that could support its habitability. But some caution is warranted when drawing conclusions about the ocean composition from the plume, since space weathering can alter plume material as it transits from the source to the spacecraft. We quantitatively evaluate the extent of this modification in terms of the H2 generated by radiolysis of plume ice grains, using a Monte Carlo model that captures both production and transport. We find that plume photoelectrons are the dominant drivers for radiolysis despite depletion of electron density by nanograin charging. Under nominal conditions, radiolytic H2 production appears to be insufficient to account for the reported H2 mixing ratio of ~1%, so the hypothesis of a hydrothermal source still stands. However, we note that our estimates are acutely sensitive to the assumed size distribution of emitted plume grains, which is not well constrained by Cassini observations. We show that, for example, a relatively high power-law exponent of 5 for the grain size distribution, which is consistent with some Cassini-based estimates, makes a radiolytic source for the reported H2 much more plausible. This demonstrates that further in-situ measurements are needed to support reliable inferences about the Enceladus ocean from observations of the exterior.

How to cite: Grayson, R. W. and Nordheim, T. A.: Exploring Exogenic Sources of Plume H2 at Enceladus, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14572, https://doi.org/10.5194/egusphere-egu26-14572, 2026.

EGU26-14742 | ECS | Orals | PS2.6

Constraining the thermophysical structure and composition of Europa’s ice shell through radar detection of eutectic interfaces 

Annie Cheng, Natalie Wolfenbarger, and Dustin Schroeder
Recently launched missions, NASA’s Europa Clipper and ESA’s JUpiter ICy moons Explorer (JUICE), are equipped with ice-penetrating radar sounders for the purpose of studying Europa’s subsurface ice shell and global ocean. Detection of a eutectic interface within Europa’s ice shell may offer a direct measurement on the amount and distribution of brine at its lowest thermodynamically stable temperature. We explore how a potential radar detection of a eutectic interface may help constrain ice shell thickness, thermal structure, and compositional chemistry. We find that the role of bulk ice shell salinity in eutectic detection differs significantly across different binary endmember compositions, NaCl and MgSO4, as well as multi-ion compositions of ice shell chemistry. We additionally find that the geometric distribution of eutectic brine impacts radar detectability, and we further discuss the prospects of detecting vertically and laterally extended hydrological features such as dikes, sills, or perched lakes.

How to cite: Cheng, A., Wolfenbarger, N., and Schroeder, D.: Constraining the thermophysical structure and composition of Europa’s ice shell through radar detection of eutectic interfaces, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14742, https://doi.org/10.5194/egusphere-egu26-14742, 2026.

EGU26-15159 | ECS | Orals | PS2.6

Inertial waves in a convecting ocean 

Daniel Abdulah and Wanying Kang

Inertia waves are considered a potential source of oceanic dissipation in deep fluid interiors such as the oceans icy satellites or the convective envelopes of stars. The geometry of a finite ocean, together with the reflecting properties of inertia waves, allows periodic paths called attractors to accumulate large amounts of energy eventually balanced by viscous dissipation. The interaction of these wave attractors with convective plumes at the pole and mid-latitudes is studied with 3D MITgcm simulations. Strong convection is found to inhibit energy accumulation along wave attractors as the inertia wave beam is decohered. A range of temperature gradients and wave beam properties is explored to approach a scaling law for the critical Rayleigh number below which inertia wave beams may be sustained.

How to cite: Abdulah, D. and Kang, W.: Inertial waves in a convecting ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15159, https://doi.org/10.5194/egusphere-egu26-15159, 2026.

EGU26-17296 | ECS | Orals | PS2.6

Serpentinisation-driven liberation of bioessential phosphite (P(III)) in Europa-relevant lithologies. 

Leanne G. Staddon, Claire R. Cousins, Abu S. Baidya, Joanna Kalita, Eva E. Stüeken, and Nick Mappin

As a plausibly habitable Solar System “ocean world”, Jupiter’s moon Europa is a key target for ongoing and future exploration [1]. A fundamental habitability requirement is the provision of bioavailable Phosphorus (P), one of six elements (CHNOPS) essential for all known life that is vital for the formation of phospholipids, the structural framework of DNA and RNA, and energy production and transfer. However, the delivery, abundance, and speciation of P into Europa’s subsurface ocean is currently entirely unconstrained.

Phosphorus is a limiting nutrient on Earth [2], as P is less abundant than other CHNOPS elements and P reservoirs are dominated by the poorly soluble phosphate (P(V) as PO43-) mineral apatite. While present at lower abundances, reduced P species phosphite (P(III)) has significantly greater solubility and reactivity, and hence bioavailability, than phosphate [2-3]. As such, phosphite has been argued to represent an important P source in early Earth and extraterrestrial aqueous environments [3-5]. Several geological pathways exist to produce and liberate phosphite. Most pertinent to Europa is serpentinisation [5], where water-rock reaction of ultramafic and mafic lithologies at the mantle-ocean interface may i) reduce lattice-bound phosphate substituting for SiO4 in olivine to phosphite and/or ii) liberate magmatic phosphite lattice-bound in Mg-Fe silicates. Though ultramafic and mafic rocks possess low bulk P contents, their likely lithological dominance in differentiated icy moons means serpentinisation is a viable mechanism for bioavailable P delivery to subsurface oceans [5].

Following the methods of [3] and using loss of ignition (LOI) as a proxy for water/rock ratios and degree of serpentinisation, we constrain P speciation in variably serpentinised ultramafic to mafic lithologies from the Troodos ophiolite, Cyprus. Preliminary data reveal variable but ubiquitous phosphite in mantle and crustal samples (P(III)/P(V) ≤0.01 to 0.45). In variably serpentinised harzburgites, increasing P(III)/P(V) correlates with LOI, supporting serpeninisation-driven liberation of phosphite, via either reduction of phosphate or preferential release of magmatic phosphite. Furthermore, an observed decrease in P(III)/P(V) above 15 % LOI supports the thermodynamic models of [5], which imply an upper limit to the water/rock ratios permissive for these reactions. These data indicate serpentinisation-driven reduction of phosphate and/or liberation of magmatic phosphite is a resolvable and ubiquitous process in natural materials analogous to Europa’s rocky ocean floor, providing further constraints on the habitability of Europa’s subsurface ocean.

[1] Vance et al. (2023), Space Science Reviews 219, 81. [2] Duhamel (2024) Nature Reviews Microbiology 23, 239-255. [3] Baidya et al. (2024), Communications Earth & Environment 5(1), 491. [4] Baidya et al. (2025) Nature Communications 16, 4825. [5] Pasek et al. (2022), GCA 336, 332-340.

How to cite: Staddon, L. G., Cousins, C. R., Baidya, A. S., Kalita, J., Stüeken, E. E., and Mappin, N.: Serpentinisation-driven liberation of bioessential phosphite (P(III)) in Europa-relevant lithologies., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17296, https://doi.org/10.5194/egusphere-egu26-17296, 2026.

EGU26-17345 | Orals | PS2.6

Inducing Fields and Lorentz force driven flows in the subsurface oceans of icy moons 

Johannes Wicht and Ilse De Langen

Because of Jupiter’s rotation and the orbital motion of the Galilean moons, the subsurface oceans experience a time varying magnetic field. This gives rise to magnetic induction of electric currents, and the measurement of the related magnetic fields lead to the discovery of the subsurface oceans. The complex orbital motions yield magnetic field variations of different frequencies, with different amplitudes and phases that both change over time. Analyzing the orbital evolution, we provide a catalogue of these important parameters, which are crucial for interpreting the measured induced magnetic fields.

The interaction of the electric currents with the magnetic field results in Lorentz forces, which drive flows in the oceans. We perform numerical simulations of this process and identify two types of induced flows: 1) persistent axisymmetric westward flows and 2) flows reminiscent of inertial modes, which are typical for the dynamics of rotating systems. An attempt to scale our simulations to the ocean properties suggests that the flow amplitudes remain much slower than convective driven flows.

How to cite: Wicht, J. and De Langen, I.: Inducing Fields and Lorentz force driven flows in the subsurface oceans of icy moons, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17345, https://doi.org/10.5194/egusphere-egu26-17345, 2026.

EGU26-18256 | ECS | Posters on site | PS2.6

Cassini Bistatic Radar Experiments on Titan’s Solid Surfaces: Progress Update on Flybys T14, T27, T34 and T124 

Giancorrado Brighi, Valerio Poggiali, Daniel Lalich, Marco Zannoni, Marco Mastrogiuseppe, Alexander Hayes, and Paolo Tortora

Between 2006 and 2016, the Cassini mission has conducted 13 downlink bistatic radar (BSR) radio science experiments of Titan’s surface. These experiments employ the High-Gain Antenna (HGA) onboard the Cassini spacecraft as transmitter and NASA’s Deep Space Network (DSN) antennas on Earth as receivers to establish a bistatic radio link bouncing off the surface of Titan. The distinct detection of X-band (λ=3.6 cm) returns from some of the observed Titan regions across different latitudes and longitudes allows to constrain surface roughness and near-surface composition based on the investigation of waveforms’ amplitude, frequency and polarization.

Solid terrains probed by Cassini BSR experiments produce heterogeneous reflections ranging from broad and weak returns to narrower and more powerful echoes or a combination of both. This is indicative of different dominant scattering mechanisms. For purely specular returns, RMS slopes and dielectric constant values—connected to near-surface structure and composition—are retrieved using a Gaussian fit applied to echo spectra, as previously done in BSR data analysis. For weaker returns, contaminated or dominated by diffuse scattering, a full scattering-model-informed fitting approach that combines specular and diffuse reflection components is applied to decuple the two contributions and more accurately characterize surface properties.

Herein, we present a progress update on the analysis of BSR experiments from flybys T14, T27, T34 and T124, highlighting regional variations in forward scattering and providing preliminary findings on surface roughness and near-surface dielectric constant of various regions on Titan. When possible, we exploit echo recordings from different, independently calibrated DSN antennas and discuss and compare BSR results with surface properties inferred from both Earth-based and Cassini (monostatic) RADAR observations.

How to cite: Brighi, G., Poggiali, V., Lalich, D., Zannoni, M., Mastrogiuseppe, M., Hayes, A., and Tortora, P.: Cassini Bistatic Radar Experiments on Titan’s Solid Surfaces: Progress Update on Flybys T14, T27, T34 and T124, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18256, https://doi.org/10.5194/egusphere-egu26-18256, 2026.

In the near future two space missions will aim to study the Galilean satellites to assess the internal structure of the icy crusts and to detect subglacial liquid water, using radar sounders. To properly interpret the radar data, it is necessary to understand the dielectric properties of the icy shells of these bodies, as they control radar signal penetration and anomaly (i.e., water) detection. The current knowledge of these properties for the types of water ices believed to be present in those moons is limited, which would potentially produce incorrect interpretations of the radar data, thus risking the scientific goals of these missions. Thanks to funded ERC Advanced grant SWIM (Surfing radio waves to detect liquid water in the solar system), we start developing new methodologies and protocols to create a groundbreaking knowledgebase that fills this critical gap. To reach this goal, we started to apply a novel methodology for conducting dielectric measurements across a wide range of frequencies (including the challenging interval used by these radar systems) and temperatures representative of the different ice-forming environments. Such measurements will be integrated with CT microtomography imaging, Raman spectra and molecular dynamic modelling, to address several unresolved questions regarding the dielectric properties of pure and doped ice.  Such pioneering research will create a wide-ranging dataset of the dielectric properties of non-terrestrial ices and will allow to obtain the maximum benefit from missions such as JUICE and Europa CLIPPER.

How to cite: Pettinelli, E.: Understanding ice dielectric properties through the SWIM project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18709, https://doi.org/10.5194/egusphere-egu26-18709, 2026.

EGU26-18896 | ECS | Posters on site | PS2.6

TRIPLE Project: From Antarctic Subglacial Lake Exploration to Icy Moon Missions 

Mia Do, Fabian Becker, Dipankul Bhattacharya, Oliver Funke, Daniel Gregorek, Dirk Heinen, Julia Kowalski, Jean-Pierre de Vera, Christoph Waldmann, and Christopher Wiebusch

In search of extraterrestrial life within our Solar System, icy moons emerge as promising candidates. Previous observations of Jupiter’s moon Europa indicate the existence of a global ocean beneath the moon’s icy shell. As there are only rare, weakly constrained plume activities on Europa compared to the Saturnian moon Enceladus, any future mission will have to penetrate the kilometer-thick ice layer in order to investigate the properties and constituents of the water in the ocean below.

Within the TRIPLE project, initiated by the German Space Agency at DLR, an advanced semi-autonomous exploration system for subglacial lakes and ocean environments is developed. The project aims to contribute to future space missions by demonstrating the following integrated system in an analogue terrestrial test. This includes a melting probe for penetrating the ice layer with a launch and recovery system to deploy a miniaturized underwater vehicle for autonomous investigation of the subsurface water reservoir. The integrated science payload is tailored to allow for detecting complex organics and assessing the potential habitability of both the ice and liquid water environments.

The operational capability of the TRIPLE system will be validated in a test campaign in Antarctica’s Dome C region. This area is of great interest due to the existence of subglacial lakes beneath a layer of ice several kilometers thick. Testing in a terrestrial analogue allows to exploit synergies with polar research, including studies of microbial communities in isolated ecosystems, interactions between ice-sheet and subglacial hydrology, and climate developments. As an intermediate step towards Dome C, the upcoming test campaign of TRIPLE is scheduled for the Antarctic Summer Season 2026/27 on the Ekström Shelf Ice near Neumayer-Station III.

In this contribution, we will present the scientific objectives and the current exploration system of this campaign, and provide an outlook on the following Dome C mission. In view of the primary scientific objectives of a future space mission to Jupiter's moon Europa, we will also comment on challenges and potentials regarding transferability of our sensors and engineering solutions to a planetary mission.

How to cite: Do, M., Becker, F., Bhattacharya, D., Funke, O., Gregorek, D., Heinen, D., Kowalski, J., de Vera, J.-P., Waldmann, C., and Wiebusch, C.: TRIPLE Project: From Antarctic Subglacial Lake Exploration to Icy Moon Missions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18896, https://doi.org/10.5194/egusphere-egu26-18896, 2026.

EGU26-19674 | Orals | PS2.6

New constraints on the composition and physical properties of the icy surface on Enceladus’ South Polar Terrain 

Gabriel Tobie, Victoria Iglesias-Munoz, Léo Scordia, Benoit Seignovert, Erwan Le Menn, Stéphane Le Mouélic, Nicolas Modé, Riccardo Artoni, Olivier Bollengier, and Gaël Choblet

The observation of active jets of ice grain and vapour emanating from four warm faults (called tiger stripes) at Enceladus’s South Pole was one of the major discoveries of the Cassini-Huygens mission (Porco et al. 2006, Spencer et al. 2006, Waite et al. 2006, Spahn et al. 2006).  Infrared mapping carried out by the Visual and Infrared Imaging Spectrometer (VIMS) on board the Cassini spacecraft provided information on surface composition, but also on the physical state (grain size and degree of crystallinity) near active faults (Brown et al. 2006, Jaumann et al., 2008; Taffin et al., 2012; Filacchione et al., 2016, Combes et al. 2018, Robidel et al. 2020). However, many spectral characteristics were not fully exploited by previous studies. Here, by acquiring laboratory infrared spectra of ice powder analogues, we identified several salt compounds, and potentially CO2 clathrate, at the surface, with a higher concentration along active faults. Our analysis shows that the spectral signatures in the inter-stripe regions are consistent with fresh, cold, fine-grained ice deposits, while ice near the tiger stripes has been thermally processed. The higher concentration of salts observed along the tiger stripes, as well as the main spectral features of water ice, imply significant sublimation and sintering processes in the vicinity of active jet sources. These new results provide essential constraints for identifying the best landing site for a future mission to Enceladus and for anticipating the mechanical properties of the icy regolith.

How to cite: Tobie, G., Iglesias-Munoz, V., Scordia, L., Seignovert, B., Le Menn, E., Le Mouélic, S., Modé, N., Artoni, R., Bollengier, O., and Choblet, G.: New constraints on the composition and physical properties of the icy surface on Enceladus’ South Polar Terrain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19674, https://doi.org/10.5194/egusphere-egu26-19674, 2026.

EGU26-19686 | ECS | Posters on site | PS2.6

Deciphering surface properties of the Jovian moons using radiative transfer modelling and NIR data 

Guillaume Cruz Mermy, Frédéric Schmidt, François Andrieu, Thomas Cornet, and Inès Belgacem

The Galilean moons are witnesses to unique physical processes and exhibit active phenomena over a wide range of timescales. They are therefore central targets of upcoming exploration missions, notably Europa through NASA’s Europa Clipper mission and Ganymede through ESA’s JUICE mission. These moons are strongly influenced by the intense electromagnetic environment generated by Jupiter and display strong coupling between their surfaces, exospheres, and the Jovian magnetosphere. The surface morphologies observed appear to result from a competition between external processes, such as space weathering [1] and micrometeorite bombardment, and internal processes, such as the upwelling of deep material [2]. The presence of subsurface water reservoirs may enable material exchange between the interiors of these moons and their external environments. This also reinforces their strong exobiological potential and raises important questions regarding their habitability. An improved understanding of the physicochemical properties of their surfaces is therefore a key step in characterising the endogenic and exogenic processes that have governed the evolution of these moons over geological timescales.


The study of surface properties is facilitated by the large volume of data obtained from both ground-based observations and spacecraft missions that have explored the Jovian system. In particular, near-infrared data (1–5 µm) are available at a range of spatial and spectral resolutions. In this study, we focus on observations acquired by JWST/NIRSpec and Galileo/NIMS. Many compounds have already been detected and mapped on these moons [3,4,5], but little is known regarding other properties, such as their grain size and porosity. To robustly estimate the microphysical surface properties, realistic radiative transfer models are required to account for the highly nonlinear scattering interactions occurring within complex surfaces. Here, we present results obtained using the Hapke model [6], considering two distinct cases: (i) a semi-infinite, single-layer granular mixture with a fixed porosity of 50%, and (ii) a two-layer model consisting of a granular medium of variable thickness and porosity overlying a semi-infinite granular substrate. To retrieve volumetric abundances, grain sizes, porosity, and the thickness of the upper layer, we employ a Bayesian inversion approach that has demonstrated its effectiveness in previous surface characterisation studies [7,8].


We present results obtained from several distinct observations of Europa’s trailing hemisphere, as well as multiple spectroscopic inversions performed on JWST observations of Europa and Ganymede. The derived results enable the production of maps of surface microphysical properties. 


[1] Carlson et al., 2005; [2] Pappalardo et al., 1999; [3] Ligier et al., 2016; [4] King et al., 2022; [5] Villanueva et al., 2023; [6] Hapke et al., 2012; [7] Cruz-Mermy et al., 2022; [8] Cruz-Mermy et al., 2025.

How to cite: Cruz Mermy, G., Schmidt, F., Andrieu, F., Cornet, T., and Belgacem, I.: Deciphering surface properties of the Jovian moons using radiative transfer modelling and NIR data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19686, https://doi.org/10.5194/egusphere-egu26-19686, 2026.

Surface properties like porosity and grain sizes on icy moons remain poorly understood, despite decades of remote sensing observations. Spaceborne instruments do not measure the ice microstructure directly: instead, they record proxy measurements (such as thermal flux or reflectance spectra) which are then interpreted through modeling to estimate thermal inertia, porosity, grain size, etc... However, from data acquisition to parameter inversion, these models rely on various assumptions and simplifications. As a result, different studies using the same raw data but distinct modeling approaches can give different estimates for the same physical parameters, making it difficult to place a robust constraint on the true surface characteristics of the ice.

This study takes a different approach by exploring the parameter space of values that are physically incompatible with icy moon conditions. Notably, the consistently low thermal inertia (<20 SI from Howett et al. 2010) measured at the very top surface of all icy moons is far below that of bulk crystalline water ice (~2000 SI). While a lower thermal conductivity could be attributed to the mix of insulating materials (e.g., dust or amorphous ice phases) regions of pure crystalline ice also exist on these bodies and yet they still present such low thermal inertia near the surface.

Through physics-based reasoning on this data, we demonstrate that pure crystalline water ice can only achieve such low thermal inertia through a combination of very high porosity (>80%), small grain sizes (<1 mm) and an unconsolidated regolith (minimal bond sizes).Tighter or looser constraints can be derived depending on the assumptions underlying the various models found in the literature, which are also discussed. By defining the range of allowed porosities and grain sizes, these constraints will help Bayesian inversion modeling in spectroscopy (Cruz-Mermy et al. 2025) including for future MAJIS (JUICE) and MISE (Europa Clipper) spectrometers, as well as for the planning of rover operations and landing site selection on such highly porous surfaces (e.g., Voyager2050, ESA’s L4 mission).

How to cite: Mergny, C.: The Low Thermal Inertia of Icy Moons: Implications on Surface Porosity, Grain Size, and Regolith Structure, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21185, https://doi.org/10.5194/egusphere-egu26-21185, 2026.

EGU26-21408 | Posters on site | PS2.6

Large volumes of eutectic brines resistant to freezing at low pressures: implications for effusive flows on icy worlds 

Mark Fox-Powell, Petr Broz, Vojtěch Patočka, Priyanka Sindhu, Rachael Hamp, Matthew Sylvest, Zoe Emerland, and Manish Patel

Icy worlds such as Europa, Enceladus and Ceres show evidence for subsurface liquids reaching the surface, either as plumes or effusive flows. Regions where this has occurred serve as potential archives of subsurface chemistry and habitability, making them prime targets for future missions. Subsurface fluids on these bodies may range in salinity from dilute to eutectic compositions, with brines approaching eutectic concentrations expected to be more common in the shallow subsurface due to their longevity at low temperatures. Despite their importance, little is understood about how highly saline fluids evolve if exposed to surface conditions.

We exposed large quantities (~50 kg) of NaCl and MgSO4 brines at eutectic concentrations to pressures below their triple points and observed their physical behavior and thermal evolution. We found that eutectic brines, if emplaced into low-pressure environments, resist evaporatively driven freezing through the formation of salts at their surface which acts to strongly decrease evaporation rate. Furthermore, instead of evolving towards the eutectic point and thus complete solidification, the salinity and temperature of the brines instead asymptotically approached their hydrate liquidus at a concentration approximately 3% above the eutectic concentration. After 120-300 minutes, both brines approached steady-state whereby salts precipitated at the surface and sank, to be replaced by fresh surficial salts. Our findings indicate that eutectic liquids could be relatively long-lived in low-pressure environments. Furthermore, although emplaced brines at icy worlds may freeze conductively from below, ice formation should not be expected in the upper 10s of cm simulated by these experiments. Instead, we predict the systems should continue to evaporate and precipitate hydrates until dryness, meaning that regions where eutectic brines have been emplaced could be indicated by salt lags rather than salt-bearing ices. Our findings provide a new perspective on surface processes involving the extrusion of high-salinity liquids into low-pressure environments and the possible longevity of liquid water under non-equilibrium scenarios on planetary surfaces.

How to cite: Fox-Powell, M., Broz, P., Patočka, V., Sindhu, P., Hamp, R., Sylvest, M., Emerland, Z., and Patel, M.: Large volumes of eutectic brines resistant to freezing at low pressures: implications for effusive flows on icy worlds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21408, https://doi.org/10.5194/egusphere-egu26-21408, 2026.

EGU26-22787 | ECS | Orals | PS2.6

Infrared Search for Vinyl Cyanide in Cassini/CIRS Polar Winter Observations 

Zachary McQueen, Conor Nixon, and Keeyoon Sung

Titan’s atmosphere is a dense and active chemical reactor forming complex organic and nitrile species relevant to prebiotic chemistry. Molecular nitrogen (N2) and methane (CH4) undergo photolysis and subsequently react to form more complex molecules that then continue this photochemical process creating a vast chemical network leading to the formation of organic hazes that give Titan its characteristic glow. Nitriles in Titan’s atmosphere, specifically, are of astrobiological interest as they make up the necessary precursors to more complex molecules, such as amino acids, necessary for the formation of life.  One nitrile species, vinyl cyanide (C2H3CN), previously detected in ALMA (Atacama Large Millimeter Array, Palmer et al. 2018) observations of Titan’s atmosphere bears significant astrobiological relevance.  Stevenson et al. (2015) reported that vinyl cyanide had the capability to form self-assembled structures that resembled cell membranes in oxygen poor environments such as Titan. Furthermore, Mayer and Nixon (2025) recently proposed a mechanical mechanism for the formation of vesicles through precipitation induced spray droplets from the surface of Titan’s methane lakes when a thin monolayer of amphiphiles such as vinyl cyanide are present. Here, we present the search for vinyl cyanide in infrared observations of Titan’s south polar limb from Cassini’s Composite InfraRed Spectrometer (CIRS). We make use of a newly obtained pseudo line list from a high-resolution measurement of the vinyl cyanide mid-infrared spectrum. Using this new spectroscopic information, we search for the  vibrational mode, centered at 682 cm-1, in CIRS observations from Cassini’s T110 flyby of Titan’s south polar limb (89 S) during the southern polar winter in March of 2015. Vinatier et al. (2018) used these observations previously to detect the infrared spectral signature of benzene ice at 680 cm-1; however, at that time, the infrared spectrum of vinyl cyanide was not well characterized. Even following the inclusion of benzene ice into the spectrum, there is still a significant residual remaining in the CIRS spectrum near 682 cm-1, indicating a missing gas in the radiative transfer model of these observations. With this detection, we can also show how vinyl cyanide is enriched at Titan’s winter pole and assess the astrobiological relevance of this key nitrile species.

References:

Palmer, M. Y. et al. ALMA detection and astrobiological potential of vinyl cyanide on Titan. Sci. Adv. 3, e1700022 (2017).

Stevenson, J., Lunine, J. & Clancy, P. Membrane alternatives in worlds without oxygen: Creation of an azotosome. Sci. Adv. 1, e1400067 (2015).

Mayer, C. & Nixon, C. A. A proposed mechanism for the formation of protocell-like structures on Titan. Int. J. Astrobiol. 24, e7 (2025).

Vinatier, S. et al. Study of Titan’s fall southern stratospheric polar cloud composition with Cassini/CIRS: Detection of benzene ice. Icarus310, 89–104 (2018).

Acknowledgement:

Portions of this research were performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration and California Institute of Technology.

How to cite: McQueen, Z., Nixon, C., and Sung, K.: Infrared Search for Vinyl Cyanide in Cassini/CIRS Polar Winter Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22787, https://doi.org/10.5194/egusphere-egu26-22787, 2026.

EGU26-22822 | Posters on site | PS2.6

Predicting the intrusion depth of a lander on the surface of Enceladus using a regolith stratification model 

Bastian Gundlach, Ben Aussel, Tina Rückriemen-Bez, Carsten Güttler, Jürgen Blum, Riccardo Atoni, Tara-Marie Bruendl, Francois Gutierrez, Martin Haag, Axel Hagermann, Jörn Helbert, Fredrik Leffe Johansson, Niels Ligterink, and Gabriel Tobie

Saturn’s icy moon Enceladus is the prime target for ESA’s fourth large-class mission (L4) [1]. In addition to placing an orbiter around Enceladus, the mission would involve deploying a lander to the South Polar Terrain of the moon. A crucial parameter to ensure safe landing is the intrusion depth of the lander on Enceladus’ icy surface. In this study, our main goal is to calculate this intrusion depth considering the structure of the ice shell of Enceladus. For this, we use an existing stratification model for granular matter [2,3], where the density of the surface layers increases with depth due to the gravity of Enceladus. We use parameters derived from compression curves of granular ice from laboratory experiments [e.g., 4], such as the turnover pressure and logarithmic transition width from loose to dense packing, as input parameters for the stratification model. Once the stratification of Enceladus’ icy surface is calculated, we predict the intrusion depth of an object (i.e., ESA’s L4 lander) resting on the surface, which compacts the porous, granular ice due to its weight. We will analyze the sensitivity of the calculated intrusion depth on the input parameters and define worst-case scenarios. Moreover, we will consider additional physical processes such as sintering [5] and will discuss next steps involving dynamic compaction.

References:

[1] Helbert et al. (2025) EPSC-DPS2025-1307. [2] Blum et al. (in revision), submitted to A&A. [3] Bürger et al. (2024), JGR: Planets, 129, e2023JE008152. [4] Lorek et al. (2016), A&A 587, A128. [5] Gundlach et al. (2018), MNRAS 479, 5272–5287.

How to cite: Gundlach, B., Aussel, B., Rückriemen-Bez, T., Güttler, C., Blum, J., Atoni, R., Bruendl, T.-M., Gutierrez, F., Haag, M., Hagermann, A., Helbert, J., Johansson, F. L., Ligterink, N., and Tobie, G.: Predicting the intrusion depth of a lander on the surface of Enceladus using a regolith stratification model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22822, https://doi.org/10.5194/egusphere-egu26-22822, 2026.

The cryospheres of ice-covered ocean worlds (i.e., their surfaces and solid ice layers) represent a new frontier in our understanding of the functioning and evolution of planetary systems. Cryospheres govern ocean-surface interaction and play active roles in the evolution and habitability of icy worlds. Furthermore, icy world cryospheres show evidence for a fascinating spectrum of geological activity that is unique to this class of world. Dynamic processes such as ‘cryovolcanic’ plumes or brine extrusions offer immense promise for exploration, as they may transport liquids from the subsurface to the surface environment where they can be studied by spacecraft. Indeed, salts and other endogenic materials have been detected at the surfaces of Enceladus, Europa, Ganymede and Ceres, indicating that some ocean to surface transport takes place. However, interpreting the archive of ocean chemistry recorded at icy world surfaces requires accounting for how the composition of ocean materials is influenced by cryosphere processes. Many of these processes have no direct analogy in silicate rocky planetary systems, meaning new frameworks are required. This challenge can be met by integrating studies of Earth’s cryosphere with laboratory simulations.

I will present results from studies of experimental and natural analogues that provide insight into the potential chemical diversity generated by dynamic processes in icy world cryospheres. I will show how permafrost-hosted brine seeps in the High Arctic can help us understand how ocean composition and evidence of habitability could be transported and altered by ice-hosted brines. I will describe laboratory investigations into how salts emplaced from subsurface fluids can influence long-term evolution of icy world surface features. Finally, I will highlight recent laboratory discoveries of novel hydrates that show how the thermal history of frozen fluids can be recorded in their mineralogical composition. Together, this work provides new frameworks for interpreting surface composition of icy worlds that can be used by upcoming missions such as NASA's Europa Clipper and ESA's JUICE to identify regions of recent fluid delivery to the surfaces of icy worlds.

How to cite: Fox-Powell, M. G.: Liquid processes within icy world cryospheres: Insights from experimental and natural analogues, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22901, https://doi.org/10.5194/egusphere-egu26-22901, 2026.

EGU26-533 | ECS | PICO | GM6.1

Inventory of young mass wasting events in Mars' Southern Hemisphere: Insights into characterization and formation mechanisms 

Deniz Yazıcı, Oguzcan Karagoz, Thomas Kenkmann, Filippo Carboni, and Tolga Görüm

Landslides are key geomorphic features on Mars that record past climate conditions, slope stability, and volatile-driven processes. We present a regional inventory of 290 landslides between 20°S and 50°S on Mars, focusing on Late Amazonian events underrepresented in global databases. To map landslides, we used high-resolution Context Camera (CTX) (5 m/px) satellite imagery, and detailed morphometric analyses were performed using stereo-derived CTX Digital Elevation Models (DEMs) (6 m/px) satellite. The mapped landslides were classified into three major types: rock avalanches, slumps, and ejecta-type features. Our results indicate that landslide areas range from 0.26 to 174 km², with estimated volumes between 0.003 and 5.72 km³. The height-to-length (H/L) ratios, varying from 0.00013 to 0.268, reveal substantial differences in mobility and formation mechanisms. Approximately 40% of landslides at high southern latitudes display morphologies suggestive of basal ice lubrication or cryosphere involvement, supporting ice-facilitated movement mechanisms. Crater size-frequency distribution (CSFD) analysis constrains absolute model ages of these landslides between 3.50 and 480 Ma (Middle to Late Amazonian), indicating repeated mass-wasting activity over extended geological timescales.

Spatial correlation analyses between landslides and glacial features such as Lineated Valley Fill (LVF), Lobate Debris Aprons (LDA), and Concentric Crater Fill (CCF) reveal a strong association between ice-bearing terrains and enhanced landslide mobility. These findings indicate that subsurface ice acted as both a stabilizing and lubricating agent, reducing basal friction while promoting high mobility under favourable thermal conditions.

These results provide the first comprehensive dataset of southern mid-latitude landslides, filling a major gap in Martian landslide inventories. The morphometric variability observed in this region demonstrates that cryosphere-substrate interactions play a crucial role in shaping Martian slope processes. Our findings underscore the complexity of mass wasting dynamics and their strong linkage to past climate fluctuations, providing new constraints on the timing and preservation conditions of buried ice deposits across Mars' recent geological history.

How to cite: Yazıcı, D., Karagoz, O., Kenkmann, T., Carboni, F., and Görüm, T.: Inventory of young mass wasting events in Mars' Southern Hemisphere: Insights into characterization and formation mechanisms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-533, https://doi.org/10.5194/egusphere-egu26-533, 2026.

EGU26-2886 | PICO | GM6.1

Formation of lunar swirls: Implications from Chang’E-1 Interference Imaging Spectrometer data 

Dawei Liu, Zhibin Li, Zongyu Zhang, Hongbo Zhang, and Chunlai Li

Lunar swirls remain one of the most enigmatic geological features on the Moon's surface. They appear as sinuous, high albedo patterns that are interwoven with “dark lanes” and stand out against the low-albedo background. Their unique spectral properties and strong correlation with lunar magnetic anomalies have attracted widespread scientific interest. The origin of lunar swirls is still debated. The prevailing solar wind deflection model suggests that pre-existing magnetic anomalies deflect incoming solar wind particles, leading to different degree of space weathering inside and outside the swirls and resulting in their distinctive spectral characteristics. As a key product of space weathering, nanophase iron (npFe0) directly reflects this differences inside and outside the swirls. In this study, we investigated the npFe0 content distribution of the swirl regions, offering a new perspective on the origin of lunar swirls.

In this study, we developed a model to estimate npFe0 content in lunar highland and maria soils using band ratio of remote sensing data based on laboratory-measured spectral data and npFe0 content of returned Apollo lunar samples. Then, this model was employed to the hyperspectral data acquired by Chang’E-1 Interference Imaging Spectrometer (IIM) to map the npFe0 content across five typical lunar swirl regions including Reiner Gamma, Mare Ingenii, Rima Sirsalis, Airy, and Firsov. Our results showed that npFe0 content in on-swirl regions is lower than that in off-swirl regions, indicating a suppressed space weathering effect within the swirl regions. Moreover, the relative npFe0 abundance between swirl dark lanes and surrounding off-swirl regions seems to be linked to different stages of space weathering. The distinct difference in npFe0 abundance between on-swirl regions and off-swirl fresh craters could be due to their different weathering processes. Additionally, we found a correlation between npFe0 abundance and the intensity of lunar magnetic anomalies in swirl regions. This indicates that the shielding effect of magnetic anomalies against solar wind particles may be influenced by the strength of the magnetic field. A potential relationship between npFe0 and OH-/H2O distributions within swirl regions also offer valuable insights into the solar wind-induced formation of lunar surface water. These findings support the hypothesis that incoming solar wind particles are deflected in swirl regions, leading to reduced space weathering on their surfaces.

How to cite: Liu, D., Li, Z., Zhang, Z., Zhang, H., and Li, C.: Formation of lunar swirls: Implications from Chang’E-1 Interference Imaging Spectrometer data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2886, https://doi.org/10.5194/egusphere-egu26-2886, 2026.

EGU26-2921 | ECS | PICO | GM6.1

Ground Verification Test for Tianwen-2 Payloads 

Chunlai Li

China's Tianwen-2 exploration mission is designed to perform comprehensive remote sensing, in-situ exploration, and sample return from the target small celestial bodies (2016HO3 and the main-belt comet 311P) through a series of operations including flyby, orbiting, landing, and sample collection. The mission will further investigate the formation and evolution of these target celestial bodies, their orbital dynamics, as well as correlations between the returned samples, meteorites, and data obtained from ground-based and remote sensing observations. Prior to the launch of the Tianwen-2 mission, we carried out comprehensive ground-based test to verify the detection capabilities of its nine onboard payloads and to assess the accuracy of the data they are designed to acquire. 

Results show that all payloads have met the predetermined test objectives, demonstrating robust detection performance and reliable data validity. The images obtained by the Asteroid Medium Angle Camera and Narrow Angle Camera deliver images with a modulation transfer function (MTF) ≥ 0.2, capable of providing high‑quality imagery for morphological studies. The Asteroid Laser Detection and Ranging achieves a measurement accuracy better than 3cm, enabling precise acquisition of three-dimensional topographic data of the asteroid surface. Spectral data obtained by the Asteroid Multispectral Camera, Visible and Infrared Imaging Spectrometer, and Thermal Emission Spectrometer show good agreement with reference measurements from standard instruments, confirming their capability to identify various minerals. The Dust Multi-properties Analyzer module of the Asteroid Dust and Volatiles Analyzer successfully measures dust‑particle size, morphology, velocity, and mass. The Volatiles Ion Trap Analyzer module of the Asteroid Dust and Volatiles Analyzer can detect no fewer than 14 gas species, with concentration measurement accuracy better than 33%. Using a dual‑probe gradient magnetic‑field measurement method, the Asteroid Magnetometer effectively suppress spacecraft magnetic interference and acquired valid magnetic-field information of the detection target. The Asteroid CoreScan Radar can achieve penetration depths of 35m and 5m for its low-frequency and high-frequency channels, respectively.

How to cite: Li, C.: Ground Verification Test for Tianwen-2 Payloads, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2921, https://doi.org/10.5194/egusphere-egu26-2921, 2026.

EGU26-5111 | ECS | PICO | GM6.1

Flow dynamics and behavioural characteristics of sublimation-driven granular flows under laboratory conditions 

Sharon Diamant, Susan Conway, Lonneke Roelofs, Matthew Sylvest, Zoe Emerland, Jonathan Merrison, Jens Jacob Iverson, Maarten Kleinhans, Jim McElwaine, Manish Patel, and Tjalling de Haas

Throughout our Solar System, erosional processes reshape the surfaces of terrestrial and icy bodies, ranging from planets and moons to asteroids and comets. One such process is mass wasting, which transports loose material downslope driven by gravity, forming slides, avalanches or flows depending on conditions. Over the past decades, the role of volatiles in their formation has been debated. Our understanding of extraterrestrial mass wasting relies heavily on Earth analogues; however, these are mostly influenced by liquid water, which is not stable on other planetary surfaces. Yet, numerous extraterrestrial landforms indicative of mass wasting occur on planetary surfaces with (seasonal) ice or frost and on slopes too gentle for dry material to move unaided.
Ice sublimation is a potentially plausible mechanism for driving extra-terrestrial mass wasting, whereby solid volatiles directly transition into vapour. This can initiate flow and reduce friction between sediment particles. However, because of the lack of terrestrial analogues and the complexity of producing a usable numerical model, the mechanics of sublimation on sediment mobilisation, particle dynamics and flow behaviour remain unclear. Here, we investigate the roles of volatiles and environmental conditions on the mobility and dynamics of sublimation-driven mass wasting and the morphology of their deposits.
Over the past two years, we created flows driven by sublimating CO2 using flume set-ups in two low-pressure chambers at the Open University (Milton Keynes, United Kingdom) and Aarhus University (Aarhus, Denmark). Ambient pressure was varied stepwise from 0.1 to 1000 mbar to cover the
environmental conditions of a broad range of terrestrial and icy bodies. The mass flows consisted of dry ice mixed with either high-density (∼ 2600 kgm−3) or low-density granular material (410 - 1300 kgm−3), the latter was utilised to simulate reduced gravity. The results show that reduced ambient pressures increase the volume flux of gas, thereby enhancing the fluidisation, flow mobility and runout length, particularly for low-density flows. This suggests that terrestrial bodies with lower surface gravity have more mobile sublimation-driven flows. The behaviour of the mass flows varied noticeably with ambient pressure, showing transitions through different fluidisation regimes, each marked by distinct features. At high pressures (> 20 mbar), we observe steady flows. In the 20 - 1 mbar range, the flows start to exhibit bubbles, surges and outbursts. Below 1 mbar, turbulent behaviour emerges with a diffuse particle suspension flowing above a dense layer. These behavioural regimes are similar to the regimes observed in fluidised bed experiments and have been recognised in snow avalanches and pyroclastic density currents on Earth. Currently, we are analysing internal particle dynamics and velocities for these regimes using particle tracking software. Our research shows that sublimation can be an effective driver for mass wasting on terrestrial bodies with low ambient pressures, low gravity and the presence of volatiles other than water, and might operate in distinct fluidisation regimes.

How to cite: Diamant, S., Conway, S., Roelofs, L., Sylvest, M., Emerland, Z., Merrison, J., Iverson, J. J., Kleinhans, M., McElwaine, J., Patel, M., and de Haas, T.: Flow dynamics and behavioural characteristics of sublimation-driven granular flows under laboratory conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5111, https://doi.org/10.5194/egusphere-egu26-5111, 2026.

EGU26-5639 | PICO | GM6.1

Fluvial to deltaic clinoforms observed by Curiosity in Gale crater’s Mount Sharp 

Gwénaël Caravaca, Nicolas Mangold, Gilles Dromart, William Rapin, Edwin S. Kite, Rebecca M. E. Williams, Stéphane Le Mouélic, Olivier Gasnault, Erwin Dehouck, Nina Lanza, Ashwin Vasavada, and Abigail Fraeman

The Curiosity rover continues its exploration of Mount Sharp, Gale crater’s ~5000 m-high sedimentary pile, and has been traversing for the past three years the Layered Sulfate unit (LSu), an interval initially characterized from orbit and thought to have recorded a global climatic transition toward the more arid conditions we observe nowadays on Mars. This unit, also informally known as the Mirador formation, is rich in sulfates and record mostly aeolian settings. Unexpectedly, the rover has also encountered numerous strata arguing for a recurring aqueous activity punctuating the overall arid, aeolian depositional environment.

Lately, Curiosity explored the “boxwork” unit, a high-interest region named after the orbital observation of “box-forming”, (deca-)meter-scale rectilinear features cropping out of the ground. Diagenetically-altered, fine-grained rocks making the most of the boxwork unit are probably of lacustrine origin, stressing out the importance of these aqueous conditions in the midst of the LSu. But when looking at the walls of this valley, made up of the Texoli, Mishe Mokwa and Cordillera buttes, we notably observe coarser-grained, erosion-resistant beds displaying a wealth of multi-scale sedimentary structures.

Among them are several occurrences of clinoform geometries that we sorted into three classes. Type 1 are characterized by inclined, sigmoidal to poorly cross-bedded strata, filling meter-scale, individualized lens-shaped bodies. Type 2 are characterized by inclined strata, sigmoidal but more cross-bedded strata. They are also observed filling lens-shaped bodies, but contrary to Type 1, these lenses are laterally stacked and cross-cutting each other’s immediate neighbor. Finally, Type 3 clinoforms occur in unconfined packages evidencing clearly sigmoidal, steeply-dipping (15-20°) and non-cross-bedded strata. While they are conformable with lower sub-horizontal layers pertaining to the bedrock, their top is mostly truncated by unconformable sub-horizontal layers. At the outcrop, the steeply dipping, sigmoidal strata also define a conspicuous lobate shape.

We interpret Types 1 and 2 clinoforms as the record of fluvial channels, with Type 1 a record of braided rivers and Type 2 a record of laterally migrating bars of a meandering river. Type 3 marks a conspicuous change and we interpret the vertical tripartite stratal pattern as bottomsets, foresets and topsets of a Gilbert-deltaic suite. These strata reflect fluvial to deltaic depositional settings with decreasing levels of energy from strictly fluvial, individual channels (Type 1), meandering channels (Type 2) and finally within a delta (Type 3).

These settings are in line with the quieter, presumably lacustrine, environment the boxwork unit’s strata likely origin from, and could represent the local sedimentary input. They contrast with the overall arid, aeolian structures observed to make most of the surrounding buttes and overall LSu. They nevertheless highlight a recurrence of humid episodes throughout the LSu. These events illustrate a more complex and unpredictable climatic pattern as Mars became colder and more arid.

How to cite: Caravaca, G., Mangold, N., Dromart, G., Rapin, W., Kite, E. S., Williams, R. M. E., Le Mouélic, S., Gasnault, O., Dehouck, E., Lanza, N., Vasavada, A., and Fraeman, A.: Fluvial to deltaic clinoforms observed by Curiosity in Gale crater’s Mount Sharp, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5639, https://doi.org/10.5194/egusphere-egu26-5639, 2026.

EGU26-7823 | ECS | PICO | GM6.1

The Effect of Sand-Mediated Non-Contact Interaction Between Barchans onTheir Steady-State Profiles 

Sofia Navarro Yabe, Kojiro Otoguro, Hirokazu Ninomiya, Masashi Shiraishi, and Hiraku Nishimori

Barchans are crescent-shaped dunes found in deserts with little sand, where winds blow continuously in one direction. They migrate in the downwind direction at speeds of several meters per year as sand eroded from the upwind slope is deposited on the downwind side. A characteristic feature of barchans is the localized sand outflow from their downwind-extending horns. Because barchans typically exist in clusters, this horn outflow can become sand inflow to barchans located further downwind, inducing sand-mediated interaction between upwind and downwind barchans.Most previous studies on barchan interaction have focused on direct contact interactions, i.e., collisions. However, it has recently been recognized that non-contact interaction mediated by sand transport can occur without collision. Studies on this type of interaction remain limited.This research focuses on non-contact sand-mediated interaction between upwind and downwind barchans. The interaction is investigated using a simplified crest line model [1]. This model is characterized by a small number of variables, which provides a distinct advantage in making theoretical analysis tractable.We obtain an analytical steady-state solution. The steady-state barchan shape is symmetric with respect to the sand supply source. The steady-state configuration consists of two parabolic solutions whose axes are laterally shifted due to sand inflow and connected at the supply source. Both the crest height of the steady-state barchan and the lateral displacement of the axes can be obtained analytically. We find that the steady-state barchan shape is determined by the migration velocity of the barchan and the sand inflow rate. In addition, the inverse proportionality between barchan height and migration velocity is theoretically confirmed in this study, a relationship well known in previous studies.The analytical solution shows good agreement with our previous numerical results. Our results provide deeper mathematical insight into non-contact sand-mediated interaction in barchan dune fields and offer a foundation for future studies on barchan collisions.

[1] L. Guignier. et al., Sand dunes as migrating strings, Physical Review E (2013)

How to cite: Navarro Yabe, S., Otoguro, K., Ninomiya, H., Shiraishi, M., and Nishimori, H.: The Effect of Sand-Mediated Non-Contact Interaction Between Barchans onTheir Steady-State Profiles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7823, https://doi.org/10.5194/egusphere-egu26-7823, 2026.

This study aims to isolate the effect of gravity on delta morphodynamics, a key uncertainty in interpreting Martian deltaic systems. Terrestrial deltas are commonly used as a framework to interpret deltas on Mars, yet the planet’s lower gravity fundamentally alters sediment transport processes and, consequently, delta morphology and evolution. Previous work has demonstrated that reduced gravity enhances net sediment transport for a given discharge and channel geometry, promoting a higher proportion of suspended sediment transport (Braat et al., 2024). However, the implications of these effects for delta morphodynamics have remained largely unexplored.

We conducted physical experiments in the Earth Simulation Laboratory at Utrecht University. Deltas were formed autonomously in a 3 cm-deep flume with a constant water (300 L/h) and sediment supply (2 L/h). Martian gravity was simulated by reducing the sediment particle weight through the use of low-density grains (nutshell particles, ~1350 kg/m³), thereby isolating sediment density as a proxy for gravitational effects. This approach generated higher mobility sediment and a greater fraction of suspended transport, consistent with expectations for Martian conditions. The resulting low-density deltas were compared to reference deltas formed with standard silica sand (~2650 kg/m³).

The experiments show that reduced sediment density leads to deltas with gentler equilibrium slopes and larger surface areas. The lower equilibrium slope requires little aggradation, and most of the sediment supply can be used for progradation. Low-density deltas also develop more pronounced levees, likely due to enhanced suspended sediment transport. These levees, together with minimal gradient advantages across the delta plain, result in reduced system dynamics: channels are more stable, and large-scale avulsions occur at relatively low frequencies. In contrast, normal-density deltas exhibit more frequent channel migration and avulsions. As a result, low-density deltas develop more irregular, multi-lobed planform geometries, whereas normal-density deltas tend to remain semi-circular or half-oval in shape.

These findings demonstrate that gravity alone can exert a first-order control on delta morphodynamics. Morphological characteristics commonly interpreted on Mars as indicators of fine grain sizes, high sediment mobility, or elevated discharges may instead arise from the effects of reduced gravity. Consequently, caution is required when interpreting Martian deltas solely based on terrestrial analogues.

 

 

How to cite: Braat, L.: Rethinking Martian Deltas: The Influence of Reduced Gravity on Delta Morphology and Evolution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11314, https://doi.org/10.5194/egusphere-egu26-11314, 2026.

EGU26-12154 | ECS | PICO | GM6.1

Slope Lineae as Potential Geologic Markers of Recent Devolatilization on Mercury 

Valentin T. Bickel, Giovanni Munaretto, Silvia Bertoli, Gabriele Cremonese, Pamela Cambianica, and Natalia A. Vergara Sassarini

Slope lineae are bright, elongated streaks on Mercury’s slopes. Along with hollows, lineae are considered one of the youngest geologic features on Mercury. Past surveys suggested a qualitative relation between lineae and subsurface volatiles, implying that lineae could be geologic markers of the recent – and potentially ongoing – release of subsurface volatiles on Mercury. However, lineae have not been systematically mapped across Mercury and no quantitative analysis of their abundance, distribution, and geostatistical properties has been conducted. In [1], we use a deep learning-driven approach to scan through ~112,000 MESSENGER images and catalog slope lineae across Mercury to a) characterize their spatial distribution as well as their morphometric and spectral properties and b) use geostatistical and change detection approaches to explore whether lineae are active today – and whether they could be tied to recent or ongoing devolatilization on Mercury. Our analysis presents several arguments for a direct link between lineae formation and devolatilization: 1) lineae appear to feature a blue spectral slope, like hollows, 2) lineae largely source from hollows and hollow-like features, 3) lineae are predominantly hosted by small, young impact craters that penetrated volcanic deposits, i.e., in a geologic context that facilitates (vertical and lateral) access to subsurface volatiles, 4) lineae tend to cluster on equator-facing slopes, 5) lineae appear to be hosted by terrain with slightly higher (modelled) bi-annual peak temperatures at the surface and at shallow depth, and 6) several lineae occur on shallow slopes well below the angle of repose of dry regolith, suggesting the presence of volatiles as a fluidizing agent (more details are presented in [1]). We do not observe any lineae activity between 2011 and 2015, such as changed or newly formed lineae, implying that lineae activity occurs below MESSENGER’s spatial resolution and/or on timescales longer than ~4 years. Devolatilization-driven lineae activity is a hypothesis that will be scrutinized by the ESA/JAXA (European Space Agency, Japanese Aerospace Exploration Agency) BepiColombo spacecraft and the SIMBIO-SYS instrument suite (Spectrometer and Imaging for MPO BepiColombo Integrated Observatory SYStem) that are expected to initiate their science investigations in early 2027.

 

[1] Bickel et al. (2026). Slope lineae as potential indicators of recent volatile loss on Mercury. Communications Earth & Environment (in press).

How to cite: Bickel, V. T., Munaretto, G., Bertoli, S., Cremonese, G., Cambianica, P., and Vergara Sassarini, N. A.: Slope Lineae as Potential Geologic Markers of Recent Devolatilization on Mercury, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12154, https://doi.org/10.5194/egusphere-egu26-12154, 2026.

EGU26-13591 | PICO | GM6.1

Secondary pyroclastic cones created by syn-eruptive wind  

Thomas J. Jones and Bartosz Pieterek

Mafic eruptions and their associated lava fountains are a widespread form of volcanism on both Earth and other planets. These eruptions typically produce scoria and spatter cones, or hybrids of the two, and both the characteristics of the associated tephra blanket and the morphology of the pyroclastic cone can forensically provide quantitative information about the eruption conditions. However, the morphology of a pyroclastic cone results from a complex interplay between syn-eruptive processes (e.g., volume of magma erupted, grain size of pyroclasts produced, syn-eruptive wind) and post-formation erosional processes. Thus, to quantitatively use cone geomorphology to inform on volcanic processes, the contribution of each of these factors must be disentangled. Specifically, here, we focus on the effect that atmospheric winds have at the time of the eruption in controlling the resultant cone morphology. We investigate Volcán del Cuervo, a pyroclastic cone in Lanzarote that has a complex morphology consisting of a distinct, elongated shape, with a second accumulation of pyroclastic material adjacent to the main crater. Here, we use an unnamed aerial vehicle to acquire a high-resolution, photogrammetrically derived digital elevation model (DEM). This DEM allows us to quantify the cone morphology and the precise location of the associated pyroclastic deposits. Samples were collected and associated grain size and density measurements were performed to characterise the pyroclastic material constituting the cone. Together, these data were then used in a ballistic trajectory model to constrain the critical wind and eruptive conditions required to form a secondary cone. Through transplanetary analogies, we conclude that secondary cone formation by this mechanism may bias remotely sensed detections of eruptive centres on planetary surfaces. Misinterpretation of these cones as separate eruptive vents would lead to an overestimation of past volcanism. Correct identification of secondary cones can instead provide direct constrains on eruption dynamics and past atmospheric conditions, including prevailing wind directions—an aspect that is particularly important in planetary environments where direct field validation remains unfeasible.

How to cite: Jones, T. J. and Pieterek, B.: Secondary pyroclastic cones created by syn-eruptive wind , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13591, https://doi.org/10.5194/egusphere-egu26-13591, 2026.

EGU26-14513 | PICO | GM6.1

Interannual variability of sand dune fluxes and the influence of dust storms across Mars 

Matthew Chojnacki, David Vaz, and Simone Silvestro

Diverse aeolian bedforms, including dunes, megaripples, and ripples, are migrating across the surface of Mars today, as driven by seasonally variable winds. While long-term sand flux and their regional boundary conditions have been well constrained for many dune fields, an understanding of annual sand transport variability (or consistency) is lacking. Here we provide a decadal-scale analysis of migration patterns for Martian aeolian dune systems and test the hypothesis that global dust storm (GDS)-related winds can influence bedform sediment fluxes.

Annual migration was assessed at select sites in High Resolution Imaging Science Experiment (HiRISE) orthoimages (0.25–1-m/pix) and digital terrain models. Displacements were recorded by manually mapping polylines along the dune crests in GIS over 3-8 Mars years’ worth of images. Sand fluxes were computed using slipface heights from the HiRISE topography, along with dune migration estimates – see Urso et al. 2017; Chojnacki et al. 2024. A total of 20 dune fields were analyzed from 85°N-45°S for Mars years (MY) 28-36, where sites were chosen based on data availability and long-term migration trends.

Migration rates for dunes ranged between 0.3-1.2-m/Earth year, with dune median heights of 6-17-m. Whereas median sand fluxes for sites ranged between 1-10-m3/m/yr over decadal-scale time periods, annual measurements may vary by an order of magnitude. The north polar erg dunes yield the highest rates despite being largely frozen and immobile during the northern autumn, winter, and spring. Here, the seasonal cap thickness and springtime defrost timing dictate how long winds can transport sand. There were notable sand flux maxima over the MY28-29 timestep and minima in MY34-35. The most notable events during these periods were the MY28 and MY34 global dust storms, which impacted the polar vortex, temperatures, and CO2 ice deposition. MARCI and HiRISE image mapping demonstrated that MY29 (early defrost) and MY35 (late) were endmembers in terms of spring defrosting. These events were attributed to the observed sand flux heterogeneity for some polar dune fields - see Chojnacki et al., 2024.

Equatorial or tropical latitude sites also showed significant deviations of sand transport rates, including during GDS years. Five dune fields showed reduced sand fluxes (33-49%) during the 2018/MY34 (~Ls 180-240°) GDS, relative to the prior year’s measurements. This reduction of nominal sand transport may be due to the depressed daytime surface temperatures or misaligned storm track directions (relative to nominal dune-forming winds) during the 2018 GDS, which were reported in the literature. In contrast, four dune fields were observed with increased fluxes (16-39%) in that GDS year. Elevated transport rates may relate to the alignment of dunes with dust storm corridors that experienced elevated wind shear or more localized factors. Finally, three sites showed no significant deviations in annual measurements, suggesting some bedforms may be in steady state in terms of sand transport. Climate factors such as global dust storms, seasonal ice cycles, and temperature variability appear to have a crucial role in sand availability and transport for Martian dunes; these factors demonstrate the complex interplay of boundary conditions on Mars.

How to cite: Chojnacki, M., Vaz, D., and Silvestro, S.: Interannual variability of sand dune fluxes and the influence of dust storms across Mars, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14513, https://doi.org/10.5194/egusphere-egu26-14513, 2026.

EGU26-15361 | ECS | PICO | GM6.1

Numerical assessment of celerity scaling laws for ice ripples in turbulent shear flows 

Diego Perissutti, Cristian Marchioli, and Alfredo Soldati
We investigate the morphodynamics of melting ice in turbulent shear flows using an interface-resolved numerical framework, with a focus on the formation and downstream propagation of quasi-2D scallops (ripples) on the ice–water interface. At high shear rates, these ripples enhance local melting and modify hydrodynamic drag [1], yet their dynamics remain unclear due to the complex coupling between turbulence, heat transfer, and melting-freezing. The ripple migration speed (celerity) provides a compact measure of the ice morphology evolution and reflects variations in heat flux, as well as in flow conditions [2]. Direct numerical simulations (DNS) are performed for a turbulent open-channel flow capped by an evolving ice–water interface. The incompressible Navier–Stokes equations are coupled with an energy equation and a phase-field formulation capable of describing melting and freezing. Simulations are carried out using a pseudo-spectral, parallel, GPU-accelerated solver [3], allowing for fully resolved turbulence and interface dynamics at high shear rates. A parametric study is conducted to assess the influence of thermal and hydrodynamic control parameters. Three Stefan numbers spanning two orders of magnitude are considered to examine the role of latent heat, while three shear Reynolds numbers (up to 1600) are simulated to quantify shear effects. The resulting ice morphologies are analyzed in terms of ripple celerity, roughness amplitude, and characteristic wavelength. The simulations reveal clear dependencies in ripple geometry and migration speed on both shear intensity and latent heat. Based on these results, we propose a scaling law for ripple celerity as a function of Reynolds and Stefan numbers. The proposed scaling is consistent with linear stability analysis [2], while extending its applicability beyond the small-amplitude limit and into low–Stefan-number regimes, providing new insights into ice morphodynamics in turbulent flows.

[1] Bushuk M., Orton P.M., Holland D.M., Stanton T.P., Stern A.A., Gray C., Laboratory observations of ice–water interface morphodynamics in turbulent shear flow, J. Fluid Mech., 841, 614–646, 2018.
[2] Hsu K.S., Locher F.A., Kennedy J.F., Forced-convection heat transfer from irregular melting wavy boundaries, J. Heat Transfer, 101(4), 598–602, 1979.
[3] Perissutti D., Marchioli C., Soldati A., Time and length scales of ice morphodynamics driven by subsurface shear turbulence, J. Fluid Mech., 1019, A34, 2025.

How to cite: Perissutti, D., Marchioli, C., and Soldati, A.: Numerical assessment of celerity scaling laws for ice ripples in turbulent shear flows, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15361, https://doi.org/10.5194/egusphere-egu26-15361, 2026.

EGU26-15988 | PICO | GM6.1

Schirmacher Oasis, Antarctica: An Earth Analog for Glaciofluvial Landforms and Process on Early Mars? 

Mohamed Ramy El-Maarry, Omar Aldhanhani, Yogesh Ray, and Aisha Alsuwaidi

 

Past studies of Martian-analogue landscapes in Antarctica have focused on the Dry Valleys [e.g., 1-3] with the goal of understanding the drivers and potential evolution of geomorphic features in predominantly “cold and dry” conditions. Here we present a new study of a Martian analogue-landscape from the seldom studied Schirmacher Oasis (SO, 70°45′30″S 11°38′40″E) which contains landlocked lakes, polygonal patterns attributed to seasonal thermal contraction and ice wedging, in addition to chloride surface deposits, and even desiccation features associated with the seasonal and long-term drying of the land-locked lakes [e.g, 4, 5]. The features of SO have been observed on Mars, including in terrains that have been dated to Early Mars (The Noachian Period, more than 3.6 Gya).

 We investigated a number of land locked lakes using drone surveys, onsite characterization, and sample collection (Figure. 1). Preliminary results indicate that Schirmacher Oasis indeed provides a potential analogy for specific terrain on Mars, namely those associated with chloride deposits in lacustrine setting. Specifically, we propose that at least a subset of these terrains on Mars may have experienced a similar evolutionary history to that observed in SO; a fluvial, lacustrine and periglacial activity in a previously glaciated area. Studying such regions could help provide new insights into the geological and climatic evolution of Mars, particularly on regional scale, and in periods of transient warming under prevalent cold/icy conditions.

Figure 1: [Top] Geomorphological map of SO adapted from [6]. The legend has been slightly modified to highlight only a few selected units that are of relevance to this study. [Bottom] Satellite view of SO from Google Earth showing the sites visited and sampled in this study.

Acknowledgments: This work was carried out under an MOU between the Indian National Center for Polar and Ocean Research (NCPOR) and the Emirates Polar Program (EPP). The scope of work and collected materials were approved under the research permit MoES/CAG-EP/2025/45-ISEAlP1/23 from the Indian Government’s Ministry of Earth Sciences in full compliance with the Antarctic Treaty. We are deeply indebted to the support throughout from NCPOR under the guidance of Dr. Thamban Meloth, including all logistical support before travel and “on the ground” by the NCPOR team and Goa and at Maitri Station.

References: [1] Marchant, D. R., & Head, J. W. (2007). Icarus, 192(1), 187–222. [2] Tamppari LK, et al. (2012). Antarctic Science. 2012;24(3):211-228.  [3] Heldmann, J. L. et al. (2013). Planetary and Space Science 85, 53-58. [4] Phartiyal, B., et al. (2011). Quaternary International 235,  128–136. [5] Dharwadkar, A., et al. (2018). Polar Science 18, 57–62. [7] Geological Survey of India (2006). Retrieved from: https://ncpor.res.in/files/40 Antarctic Exp/Schirmacher Oasis map.pdf. 

How to cite: El-Maarry, M. R., Aldhanhani, O., Ray, Y., and Alsuwaidi, A.: Schirmacher Oasis, Antarctica: An Earth Analog for Glaciofluvial Landforms and Process on Early Mars?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15988, https://doi.org/10.5194/egusphere-egu26-15988, 2026.

EGU26-18079 | ECS | PICO | GM6.1

Beyond Size Sorting - Shape segregation in aeolian megaripple 

lior saban, Itzhak Katra, and Hezi Yizhaq

Aeolian megaripples develop on bimodal sands and are stabilized by an armoring layer enriched in coarse grains that developed on the crest. While size-selective transport is central to the segregation mechanism involved in megaripple formation, recent field observations indicate that shape segregation may also contribute to megaripple formation (Saban et al, Geosci. Lett., 2025). Here, we quantify the shape contrast between fine and coarse fractions of megaripples across multiple sites worldwide and investigate the physical mechanism that may explain it. Additionally, we investigate how ripple formation is affected by shape segregation through controlled wind tunnel experiments.

We analyzed samples from megaripple crests at multiple sites. Each sample was divided into sub-samples of fine fraction (<355µm) and a coarse fraction (>710µm), which represent the bimodal grain size distribution (GSD) of all the samples. Grain shape was quantified using a Circularity index (isoperimetric quotient), computed from a 2D projected grain outline derived from microscopy images. Grain outlines were produced by automated segmentation and were manually validated to ensure accuracy. Mineralogical composition and GSD were also measured and used as proxies for mechanical durability and abrasion history contrasts between the size fractions.

Across most sites, the coarse fraction is more angular (less circular) than the fine fraction, indicating a robust shape contrast between size fractions. To explain this pattern, we used a physically motivated combined index that accounts for the size contrast and the quartz contrast between the fine and coarse fractions. Sites where the fine grains are both relatively finer and more quartz-rich compared to the coarse fraction show a stronger shape contrast (i.e., fines are more circular). This suggests that abrasion history and mechanical durability influence grain shape.

Finally, we designed a wind tunnel experiment to isolate the role of shape segregation in the formation of nascent megaripple. We used mixtures of angular natural sand and spherical glass beads with the same grain size. These mixtures were subjected to wind above the fluid threshold until ripple formation. Spatial distribution analysis of grain shape at the end of the experiments reveals clear sorting patterns, driven solely by shape segregation, where angular grains accumulate on the crest and form an armoring-like layer.

How to cite: saban, L., Katra, I., and Yizhaq, H.: Beyond Size Sorting - Shape segregation in aeolian megaripple, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18079, https://doi.org/10.5194/egusphere-egu26-18079, 2026.

EGU26-20367 | ECS | PICO | GM6.1

Investigating the formation conditions of glacier-like forms using Bayesian inversion.  

Mórrigan Jones, Lydia Sam, Donal Mullan, Brice Rea, and Anshuman Bhardwaj

Glacier-like forms (GLFs) are one subtype of glacial features found on the Martian surface. They are located within the mid-latitudes of Mars (30-60 degrees) in both hemispheres. These features having formed within the Amazonian period during a period of higher obliquity than Mars' is at today which allowed for the preferential accumulation of icy material in the mid-latitudes. While previous studies have investigated the geographic controls on GLF formation, their former extent, and their former dynamics (Souness, et. al., 2012; Brough, et. al. 2016, 2019), the boundary conditions under which GLFs formed remain poorly constrained, particularly on a local-scale.

Our primary aim is to improve our understanding of how Martian GLFs formed and evolved with respect to their climactic and geomorphological setting using terrestrial rock glaciers as analogues. As there is still ongoing debate as to the formation dynamics of rock glaciers on Earth, be they permafrost-derived or derived from debris-covered glaciers, with the issue being that both start points can adequately describe the end-state of palaeo rock glaciers, we need to take an approach which acknowledges this issue of equifinality. Bayesian inversion is one such method that can do this. We start with the assumption that these GLFs represent permafrost-derived ice bodies where ground-temperature is a key boundary-condition for their formation. With this method, we use observed glacier geomorphology to reconstruct the former extent, volume, and thickness of the GLF to compute a posterior probability distribution for ground temperatures that are physically consistent with the reconstructed geometry of the palaeo glacier. We also consider near-surface air temperature as a secondary factor in accumulation feasibility. 

Here we present our ongoing work in this effort. We manually demarcated the geomorphological constraints of multiple GLFs on Mars within GIS software based on identifiable geomorphology within the orthorectified imagery that mark the former maximum extent of the glacier, and extract morphometric data using the georeferenced HiRISE DEM. We then used the perfect-plasticity approximation to reconstruct palaeo ice-thicknesses and volume of the palaeo glacier. These morphometrics are then compared with modelled outputs for glacier deformation, employing Bayesian logic to constrain a boundary range of long-term mean ground temperature that would be compatible to produce the reconstructed glacier morphology. We also investigate several terrestrial rock glaciers in order to assess the accuracy and validity of our approach against measurable analogue examples, which further enables us to compare the dynamics of terrestrial and Martian glaciers.

References:

Brough, Stephen, Bryn Hubbard, and Alun Hubbard. 2016. “Former Extent of Glacier-Like Forms on Mars.”, Icarus 274 (August): 37–49. https://doi.org/10.1016/j.icarus.2016.03.006.

Brough, S., Hubbard, B., & Hubbard, A. (2019, 02). Area and volume of mid latitude glacier-like forms on mars. Earth and Planetary Science Letters, 507 , 10–20. Retrieved from https://linkinghub.elsevier.com/retrieve/pii/S0012821X18306903 doi: 10.1016/j.epsl.2018.11.031

Souness, Colin, Bryn Hubbard, Ralph E. Milliken, and Duncan Quincey. 2012. “An Inventory and Population-Scale Analysis of Martian Glacier-Like Forms.” Icarus 217 (1): 243–55. https://doi.org/10.1016/j.icarus.2011.10.020.

How to cite: Jones, M., Sam, L., Mullan, D., Rea, B., and Bhardwaj, A.: Investigating the formation conditions of glacier-like forms using Bayesian inversion. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20367, https://doi.org/10.5194/egusphere-egu26-20367, 2026.

The atmospheric boundary layer (ABL) over mountainous terrain plays an important role in modulating the exchange of momentum, heat, and moisture between the surface and the free atmosphere. Unlike flat terrain, where boundary layer dynamics are relatively homogeneous, the mountain boundary layer (MoBL) exhibits pronounced heterogeneity driven by the complex interplay of multiscale orographic features. These interactions generate a broad spectrum of atmospheric motions, from turbulent eddies and coherent thermals to thermally and dynamically induced slope and valley flows. Understanding this complexity is essential for improving weather prediction, climate modeling, and air quality assessment in mountainous regions. This study investigates the structure and dynamics of the convective boundary layer (CBL) over highly complex terrain during a TEAMx test flight on 18 September 2024. Specifically, we address the following questions: What are the dominant characteristics of coherent structures in the CBL? How stationary are these features in space and time? What is their diurnal cycle? How does the model compare to observations?

To address these questions, we employ the ICON model in large-eddy simulation (LES) mode at a horizontal resolution of 65 m, using a nested domain configuration (520 m to 65 m) to capture processes across scales. The simulation domain encompasses a region around the Sarntal Alps, one of the TEAMx target areas. The ICON-LES results are compared with novel airborne wind measurements obtained during a test flight of the AIRflows system aboard the TU Braunschweig Cessna F406 research aircraft. AIRflows delivers high-resolution, three-dimensional wind profile measurements along the aircraft track, providing a unique opportunity to validate and evaluate the LES output in real atmospheric conditions. Preliminary results reveal a complex, spatially variable CBL structure with persistent thermal features and localized regions of enhanced turbulence. The comparison with AIRflows data confirms the presence and spatial organization of key dynamical structures captured by the model, while also highlighting discrepancies that inform model improvement. This work contributes to a deeper understanding of the CBL in mountainous regions and demonstrates the value of combining advanced numerical simulations with targeted airborne observations for model validation and process studies.

How to cite: Schmidli, J. and Gasch, P.: Structure of the convective boundary layer over complex terrain: ICON-LES and high resolution 3D wind observations during a TEAMx test flight, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1856, https://doi.org/10.5194/egusphere-egu26-1856, 2026.

EGU26-4439 | PICO | AS1.25

Synergistic Observations of Flow in Complex Terrain: Integrating Lidar and Drones During the TEAMx Campaign 

Norman Wildmann, Almut Alexa, Francesca Lappin, Andrea Wiech, and Alexander Gohm

Atmospheric boundary layer (ABL) dynamics in complex terrain are inherently three-dimensional, where microscale turbulence plays a critical role in driving larger-scale flow evolution. With numerical weather prediction models approaching sub-kilometer resolutions, it is increasingly important to challenge and validate the models on the small scales with high-resolution observations. Contributing to the TEAMx goal of understanding scale interactions, we present results from an intensive field experiment conducted at the Nafingalm, a pasture at the valley head of a tributary to the Inn Valley (Austria).

The experimental site, a north-south aligned valley system approximately 2x2 km wide and 500 m deep, was instrumented during the Summer 2025 Extended Observation Period (EOP). The setup included two scanning lidars, a profiling lidar, and a network of ground-based meteorological stations. These continuous observations were augmented by the SWUF-3D fleet of multicopter drones (aka Uncrewed Aircraft Systems, UAS) between 1 and 23 July 2025. Up to 30 UAS were operated simultaneously, reaching heights of 220 m above the valley floor to collect distributed measurements of 3D wind, temperature, humidity, and pressure in regions inaccessible to traditional instrumentation.

While continuous lidar scanning mapped the along- and cross-valley flow, the UAS fleet provided direct in situ validation of the assumptions required to derive turbulence statistics from remote sensing. Furthermore, the spatial distribution of the drones allows for direct measurement of shear contributions, buoyancy, and advective tendencies. We present preliminary analyses of two contrasting Intensive Observation Periods (IOPs): one characterized primarily by thermally driven flow and another with increased mesoscale forcing. These cases highlight the strength of synthesizing remote sensing with distributed UAS measurements to resolve scmall-scale dynamics in complex terrain.

How to cite: Wildmann, N., Alexa, A., Lappin, F., Wiech, A., and Gohm, A.: Synergistic Observations of Flow in Complex Terrain: Integrating Lidar and Drones During the TEAMx Campaign, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4439, https://doi.org/10.5194/egusphere-egu26-4439, 2026.

EGU26-4800 | ECS | PICO | AS1.25

Linking valley flow and vertical exchange in complex terrain – the LIVAVERT(EX)2 project 

Philipp Gasch and Loren Schaeffler

Quantifying the exchange of mass, momentum and energy between the earth’s surface and the atmosphere is pivotal for the understanding and prediction of weather and climate processes. Due to the superposition of horizontal and vertical transport, exchange processes in complex terrain are especially efficient and important.

This contribution presents a new project embedded in the international TEAMx campaign. The LIVAVERT(EX)2 project - linking valley flow and vertical exchange in complex terrain - focuses on observing exchange processes in the Sarntal Alps region, a local hotspot of convection initiation in the Alps. As part of the project, a novel airborne Doppler lidar (ADL) is deployed for the first extended measurements in complex terrain. Thereby, 3D wind observations are available at 100 m along-track and vertical resolution, providing spatially resolved insight into valley wind systems and vertical exchange. The variability observed across repeated flights enables the differentiation between recurring and transient features.

TEAMx also encompasses a KITcube deployment in the Sarntal Alps region, which establishes an extensive meso-scale ground-based Doppler lidar (GDL) network. Through the comparison of ADL and GDL observations of valley flow, the Doppler lidar wind profiling accuracy and representativeness can be validated. Additionally, new ways to validate existing GDL-based volume flux estimation methods are created. Combining volume flux budget and direct vertical exchange observations allows a more quantitative insight into valley flow and its relation to convective initiation over the surrounding mountains than ever before. Overall, the LIVAVERT(EX)2 project aims to improve our understanding and the prediction of atmospheric processes in complex terrain.

How to cite: Gasch, P. and Schaeffler, L.: Linking valley flow and vertical exchange in complex terrain – the LIVAVERT(EX)2 project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4800, https://doi.org/10.5194/egusphere-egu26-4800, 2026.

EGU26-5662 | ECS | PICO | AS1.25

First Results from HEFEXIII - current state of the Hintereisferner boundary layer 

Leopold Schlagbauer, Ivana Stiperski, Alexander Georgi, Tobias Sauter, and Lindsey Nicholson

In the greater TEAMx framework and following HEFEX in 2018 and HEFEXII in 2023, the third HinterEisFerner EXperiment (HEFEXIII) took place in August and September 2025 on Hintereisferner glacier, Tyrol, Austria. During one month, a 9 m tower was deployed on the glacier, equipped with high-frequency measurements of three-dimensional wind components and temperature at five levels (0.5 m, 1 m, 3 m, 5 m and 9 m), as well as low-frequency measurements of two-dimensional wind components, temperature, and relative humidity at three additional levels (2 m, 4 m and 7 m). Furthermore, two lidar systems and a swarm of drones strategically measuring at various locations along the glacier axis, were used to assess the flow conditions in the atmosphere above the glacier. This dataset enables an evaluation of boundary-layer characteristics close to the surface while relating them to the flow in the larger mountain boundary layer above.
Here, we describe the general meteorological conditions observed during the campaign, as well as the turbulence characteristics. We contrast periods with an undisturbed boundary layer with conditions characterised by external disturbances, such as thermally driven upvalley winds or mountain waves on the glacier boundary layer and their influence on the katabatic flow. We focus specifically on vertical profiles of temperature and wind obtained during one of the drone IOPs, as well as the average turbulent fluxes of momentum and heat, and the budget terms of the turbulent kinetic energy at the different measurement heights. 

How to cite: Schlagbauer, L., Stiperski, I., Georgi, A., Sauter, T., and Nicholson, L.: First Results from HEFEXIII - current state of the Hintereisferner boundary layer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5662, https://doi.org/10.5194/egusphere-egu26-5662, 2026.

EGU26-7284 | ECS | PICO | AS1.25

The Role of Horizontal Shear Production in Hectometre-Scale WRF Simulations over Alpine Terrain 

Elias Wahl, Gionata Freddi, Alexander Gohm, Andreas Platis, Moritz Kippenberger, and Manuela Lehner

Traditional planetary boundary layer (PBL) parametrisations in numerical weather prediction (NWP) models assume horizontally homogeneous conditions. Under this assumption, one-dimensional (1D) PBL parametrisations are used, which only consider vertical mixing and neglect horizontal shear production in the prognostic turbulent kinetic energy (TKE) equation used by 1.5-order parametrisations. However, as high-performance computing capabilities continue to improve, NWP model resolutions are reaching the hectometre scale, resolving more surface features and smaller atmospheric processes, thus increasingly violating the 1D PBL assumption. This is especially true in complex terrain, where, for example, thermally driven circulations create persistent slope and valley winds characterised by intense shear in both horizontal speed and direction.

We set up nested simulations with the Weather Research and Forecasting (WRF) model for the Inn Valley, Austria, down to a hectometre-scale resolution using a modified PBL parametrisation that introduces an additional tendency for horizontal shear production into the TKE equation. This helps to account for horizontal heterogeneity in the atmosphere induced by local flow processes and acts as an intermediate step towards a complete representation of horizontal wind shear.

During the TEAMx 2025 summer Extended Observation Period (sEOP), uncrewed aircraft systems (UAS) measured vertical profiles – including TKE and turbulent fluxes – at multiple locations along a transect across the Inn Valley. Complementary radiosoundings and remote-sensing measurements captured mean wind and temperature profiles at various locations along the valley. These observations allow us to evaluate modelled vertical and horizontal wind shear, as well as turbulent properties. Results using the modified PBL parametrisation are compared with those using the traditional PBL parametrisation, which does not take into account horizontal wind shear.

How to cite: Wahl, E., Freddi, G., Gohm, A., Platis, A., Kippenberger, M., and Lehner, M.: The Role of Horizontal Shear Production in Hectometre-Scale WRF Simulations over Alpine Terrain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7284, https://doi.org/10.5194/egusphere-egu26-7284, 2026.

Mesoscale numerical weather prediction (NWP) models typically employ planetary boundary layer (PBL) schemes to represent subgrid-scale turbulence, including 1.5-order parameterizations that explicitly predict turbulent kinetic energy (TKE). One crucial assumption of these models is that horizontal gradients, such as horizontal shear, can be neglected in the TKE tendency terms. This assumption may not hold in complex terrain, where the interaction between terrain-induced flows and the orography itself can create substantial horizontal mixing.

We investigate this limitation using a high-resolution (Δx=500 m) WRF model simulation employing the traditional 1.5-order Mellor–Yamada–Nakanishi–Niino (MYNN) PBL scheme. We focus on a valley wind case in the Inn Valley, Austria, which occurred on 29 June 2025 during the TEAMx campaign. The event was characterized by clear skies and weak synoptic forcing, favoring the development of a convective boundary layer and thermally driven daytime up-valley winds with substantial mechanical mixing.

The simulations are compared against observational data from four Doppler wind lidars and several ground measurement stations in the valley. The evolution of the wind system is represented reasonably well by the model, but the peak strength of the valley wind is underestimated. Observations from one of the lidars show that the PBL scheme appears to underestimate TKE when the turbulence is dominated by mechanical production. This bias may result from the lower wind speeds or an incomplete representation of TKE production in the PBL scheme, with potential interactions between the two factors. An estimate of the horizontal subgrid-scale diffusion suggests that accounting for the currently neglected horizontal shear production in the TKE equation could lead to an improved TKE representation.

How to cite: Freddi, G., Gohm, A., Wahl, E., and Lehner, M.: Underestimation of Mechanically Generated Turbulence in a Traditional PBL Scheme over Complex Terrain: A TEAMx Case Study for the Inn Valley, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7862, https://doi.org/10.5194/egusphere-egu26-7862, 2026.

EGU26-9639 | PICO | AS1.25

Anisotropy scaling of a sloping glacier boundary layer 

Samuele Mosso and Ivana Stiperski

Glacier boundary layers present an ideal atmospheric laboratory for studying persistently stable boundary-layer dynamics over inclined surfaces. On glaciers in summer, turbulence is strongly controlled by the katabatic flow dynamics that is intimately coupled with very stable stratification at the glacier surface and the slope angle. In these kind of conditions, the basic assumptions of Monin–Obukhov Similarity Theory (MOST) are rarely met, due to the significant flux divergence, and the imposition of an alternative limiting scale. Still, bulk approaches based on MOST have shown good agreement under very stringent conditions, while alternative scaling approaches that add the slope angle into the scaling parameter, or use jet maximum height have shown promise in providing scaling frameworks for such flows.

Here we use a dense network of atmospheric turbulence observations during the HEFEX II campaign, that took place on the Hintereisferner Glacier, Austria in 2023. The campaign features ten turbulence towers with multi-level observations, distributed across the entire glacier surface (from the accumulation area to downstream of the glacier tongue) and therefore experiencing different flow conditions (katabatic flow depth) or slope angles. We focus on the mathematical invariant representing turbulence anisotropy that has recently been used to extend MOST to more realistic terrain conditions. Focusing on the flux-variance relations we show that katabatic flows over glaciated terrain display distinct turbulence characteristics at varying degrees of anisotropy that differ considerably to the previous studies over non-glaciated terrain. These peculiarities are further examined to isolate the difference between katabatic and canonical flows in terms of their flow anisotropy. We also test alternative scaling approaches, including those based on the katabatic jet height, local terrain slope, and formulations designed to avoid the self-correlation that is shown to be an issue in very stable stratification.

How to cite: Mosso, S. and Stiperski, I.: Anisotropy scaling of a sloping glacier boundary layer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9639, https://doi.org/10.5194/egusphere-egu26-9639, 2026.

EGU26-9768 | PICO | AS1.25

Flow Regimes and Turbulence Structure on a Steep Slope in Winter: Findings from the TEAMx wEOP 

Ivana Stiperski, Christophe Brun, Mauro Ghirardelli, Alexander Gohm, Mathias Rotach, and Manuela Lehner

During the TEAMx winter EOP, an extensive measurement campaign took place on a steep undulating slope in the Inn Valley, Austria. This six-week long campaign featured a suite of instrumentation, including a network of eight turbulence towers installed at two across-slope and an along-slope transects equipped with two levels of sonic anemometers, nano-barometers, and slow response sensors. In addition, four component radiation at two heights measured radiative flux divergence at a central location on the slope, a short-range Doppler wind lidar (Wind Ranger) at the bottom of the slope recorded wind speed and direction, while a fibre optic array at one along-slope and two-across slope transects, and two vertical sections complemented the set-up. Additional observations during intense observational periods included temperature profile measurements using a drone and wind speed and temperature observations using tethered balloon at the top of the slope.

Here we present the measurement campaign design and focus on the first results that highlight the spatio-temporal variability of the flow on the slope, tightly coupled with the synoptic forcing. During conditions of low synoptic forcing, persistent katabatic flows developed on the slope with acceleration down the slope and warmer conditions towards one side of this non-uniform slope. On the other hand, during foehn conditions, very large differences in the mean and turbulence characteristics can be observed between the upper across-slope transect and lower stations that are more exposed to foehn. These differences translate to distinct behaviour of similarity scaling relations, as well as the importance of different terms in the momentum and TKE budgets. 

How to cite: Stiperski, I., Brun, C., Ghirardelli, M., Gohm, A., Rotach, M., and Lehner, M.: Flow Regimes and Turbulence Structure on a Steep Slope in Winter: Findings from the TEAMx wEOP, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9768, https://doi.org/10.5194/egusphere-egu26-9768, 2026.

EGU26-11044 | ECS | PICO | AS1.25

Validation of High-Resolution ICON-LES Using Observations from HEFEX II and HEFEX III Field Campaigns 

Alexander Georgi, Tobias Sauter, and Leopold Schlagbauer

High-resolution numerical weather prediction (NWP) models are increasingly being used to study the interactions between the atmosphere and glaciers in complex alpine terrain. However, their performance under these conditions has not been sufficiently confirmed by observations, especially at a dekameter scale. This study comprehensively validates the Large-Eddy Simulation (LES) configuration of the ICOsahedral Nonhydrostatic (ICON) model using observations from the HEFEX II (2023) and HEFEX III (2025) field campaigns. Both campaigns included four weeks of intensive observations at Hintereisferner in the Ötztal Alps and were part of the international TEAMx research program, which studies multi-scale transport and exchange processes in mountainous environments.

HEFEX II focused on characterizing the spatial gradients and temporal variability of surface-layer variables, such as temperature, humidity, and wind. HEFEX III utilized coordinated UAV-based vertical profiling in combination with multiple on-glacier lidar systems to resolve atmospheric flow fields and wind patterns within the valley. Together, the two campaigns provide a unique and unprecedented observational dataset in complex glacierized terrain, offering an exceptional basis for model evaluation.

ICON-LES was applied in a one-way nested configuration, achieving a target horizontal resolution of 51 meters over the study area. We assessed model performance using qualitative and quantitative validation approaches, particularly emphasizing the model’s ability to reproduce the spatio-temporal variability of key atmospheric parameters across surface and boundary-layer scales. The results demonstrate strong agreement between ICON-LES simulations and multi-platform observations, indicating that the model realistically captures flow structures and variability in a high alpine glacier environment.

These findings support the use of ICON-LES as a reliable tool for studying atmosphere-glacier interactions and lay the groundwork for future climate impact and feedback studies in complex terrain. At the same time, the analysis highlights the current limitations of high-resolution numerical modeling and emphasizes the importance of using advanced observational techniques and large-eddy simulations together to improve our understanding of processes in mountainous regions.

How to cite: Georgi, A., Sauter, T., and Schlagbauer, L.: Validation of High-Resolution ICON-LES Using Observations from HEFEX II and HEFEX III Field Campaigns, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11044, https://doi.org/10.5194/egusphere-egu26-11044, 2026.

EGU26-12279 | PICO | AS1.25

Lidar-based observations of flow regimes and turbulence in a small Alpine valley during TEAMx 

Alexander Gohm, Norman Wildmann, Almut Alexa, and Andrea Wiech

The summer Extended Observation Period (sEOP) of the 2025 TEAMx observational campaign provided a unique opportunity to investigate multi-scale interactions in the mountain boundary layer (MoBL) and enhance our understanding of its structure and turbulent processes. In this study we present a preliminary analysis of observations from two Doppler wind lidars operated in the Weer Valley (Nafingalm, Austria) from 6 June to 24 July 2025. The focus is on 12 Intensive Observation Periods (IOPs) for which complementary airborne observations are available (June 29 and July 2, 5, 9, 11, 13, 15, 18, 19, 20, 22, and 23), though the latter are not included in this initial study. The aim is to characterize observed events by classifying different flow regimes and turbulent features, primarily using Doppler wind lidar data supported by a weather station network. This classification provides a framework for future in-depth studies and large-eddy simulations. Emphasis is placed on identifying recurring scale interactions between local and regional flows—such as valley winds and cross-mountain flows—and the resulting processes, including flow separation, waves, and shear-flow instabilities. Finally, initial turbulence metrics are calculated to support the event classification.

How to cite: Gohm, A., Wildmann, N., Alexa, A., and Wiech, A.: Lidar-based observations of flow regimes and turbulence in a small Alpine valley during TEAMx, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12279, https://doi.org/10.5194/egusphere-egu26-12279, 2026.

EGU26-13553 | PICO | AS1.25

Investigating the surface energy balance closure over mountain areas: results from the INTERFACE project 

Lorenzo Giovannini, Sebastiano Carpentari, Martina Destro, Dario Di Santo, Manuela Lehner, Roberto Monsorno, Mathias W. Rotach, Mira Shivani Sankar, Beth Saunders, Mohammadamin Soltaninezhad, Stefano Tondini, Nadia Vendrame, and Dino Zardi

This contribution presents an overview of the activities and results of the INTERFACE project, which aims to quantify the non-closure of the surface energy balance across various Alpine sites, where processes related to the lack of closure, i.e., advection due to the development of thermally-driven circulations, are expected to be particularly significant. This objective is addressed by combining flux station and unmanned aerial system (UAS) measurements. The UAS provides spatially distributed observations around eddy-covariance sites, which are essential for estimating advection.

The analysis of eddy-covariance data from various sites representing diverse Alpine contexts (e.g., valley floor, slope, and mountain top) and climatic settings (North vs. South of the main Alpine crest) allows a systematic quantification and comparison of the characteristics of the surface energy balance, including the lack of closure. Particular emphasis is placed on the evaluation of the role of thermally-driven circulations in the non-closure of the surface energy balance, utilizing objective criteria to select days with well-developed slope and valley winds.

The INTERFACE project contributes to the TEAMx international research programme, which aims to improve our understanding of exchange processes in the atmosphere over mountains.

How to cite: Giovannini, L., Carpentari, S., Destro, M., Di Santo, D., Lehner, M., Monsorno, R., Rotach, M. W., Sankar, M. S., Saunders, B., Soltaninezhad, M., Tondini, S., Vendrame, N., and Zardi, D.: Investigating the surface energy balance closure over mountain areas: results from the INTERFACE project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13553, https://doi.org/10.5194/egusphere-egu26-13553, 2026.

EGU26-18348 | ECS | PICO | AS1.25

The observational effort for characterising turbulence and transport processes on the pre-Alpine range of Monte Baldo during the TEAMx Observational Campaign.  

Giorgio Doglioni, Sebastiano Carpentari, Lorenzo Giovannini, and Dino Zardi and the Monte Baldo partners

We present the intensive field campaign conducted from mid-June to mid-October 2025 on Monte Baldo (Italian Pre-Alps) within the TEAMx programme, aimed at improving process understanding and model representation of mountain boundary-layer exchanges. This effort was driven by the DECIPHER project, which aims at disentangling mechanisms controlling atmospheric transport and mixing processes over mountain areas at different space- and timescales.

Measurements targeted a steep (~25°), east-facing, grass-covered slope in the southern Monte Baldo range, selected for its regular topography and pronounced diurnal cycle of thermally driven slope winds. The setting also enables investigation of coupling at the mountain–plain interface, linking local slope circulations to the adjacent lowland atmosphere in the Po Valley.

A coordinated suite of instruments captured processes from the surface layer to the lower troposphere and their interactions across scales. Near-surface thermodynamic variability and turbulent exchange were monitored using multi-level flux towers and a slope-wide network of thermohygrometers. Variability in aerosol and particulate matter was measured using co-located mass and optical sensors. Along- and cross-slope winds were observed with multiple wind lidars, while boundary-layer and lower-tropospheric profiles were obtained with a tethered balloon system and a Raman lidar. The surface heat budget was characterized using radiation measurements together with soil temperature and moisture observations. Complementary observations included high-frequency near-surface turbulence profiling and distributed soil-moisture monitoring using a cosmic-ray neutron sensor.

This contribution details the observational setup, characterizes the regional setting, and illustrates the potential of the dataset for evaluating slope-wind structure and the associated surface fluxes, boundary-layer mixing, and exchange pathways between mountains and adjacent plains.

How to cite: Doglioni, G., Carpentari, S., Giovannini, L., and Zardi, D. and the Monte Baldo partners: The observational effort for characterising turbulence and transport processes on the pre-Alpine range of Monte Baldo during the TEAMx Observational Campaign. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18348, https://doi.org/10.5194/egusphere-egu26-18348, 2026.

EGU26-20048 | ECS | PICO | AS1.25

Dual Radiosonde Soundings of Gravity Wave Breaking over the Alps during the 2025 Winter TEAMx Observational Campaign 

Timothy Banyard, Neil Hindley, Andrew Orr, Corwin Wright, Siddharth Gumber, and Andrew Ross
The TEAMx programme provides us with a unique observational data set which is extensive in spatial and temporal coverage and encompasses a diverse range of measurement techniques. A campaign such as this is ideal for studying the fine-scale behaviour of orographic gravity waves, including their generation, propagation and eventual breaking. As future weather and climate models are run at progressively higher resolutions, it is critical that these waves are simulated accurately across all spatial scales. Notably, regions of high vertical wind shear can lead to errors in the modelled behaviour of these waves which cause misrepresentations in both the altitude and magnitude of gravity wave drag. Furthermore, the partitioning between resolved and parameterised gravity wave drag should vary inversely across spatial scales and with consistency between different numerical models, such that the total drag remains constant. Whilst this is yet to be achieved, TEAMx has the potential to bring this closer to reality.
 
Here, we present results from the UK-funded TEAMx-FLOW project, which focuses on analysis of dual radiosonde launches during the winter extended observational period (wEOP). We analyse and quantify mountain wave momentum transport in these measurements, including using cross-spectral analysis of balloon pairs to obtain scale separation of observed waves. We also explore observations of partial wave breakdown in directionally sheared flow, a process which is not currently considered in parameterisation schemes. We will use our results to validate MetUM simulations, and hope that this research will be able to inform the development of scale-aware models in the future.

How to cite: Banyard, T., Hindley, N., Orr, A., Wright, C., Gumber, S., and Ross, A.: Dual Radiosonde Soundings of Gravity Wave Breaking over the Alps during the 2025 Winter TEAMx Observational Campaign, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20048, https://doi.org/10.5194/egusphere-egu26-20048, 2026.

EGU26-20164 | ECS | PICO | AS1.25

Measuring Horizontal Shear and Turbulence in Mountain Valleys using UAS and Lidar 

Moritz Kippenberger, Martin Schön, Marisa Ruhl, Elias Wahl, Gionata Freddi, Alexander Gohm, Manuela Lehner, Jens Bange, and Andreas Platis
Turbulent mixing in complex terrain remains a major source of uncertainty for weather and climate models. Many processes within the planetary boundary layer (PBL) occur on spatial scales that numerical models cannot resolve explicitly and thus require parameterization. For complex terrain, however, the common mesoscale-model assumption that horizontal shear production of turbulent kinetic energy (TKE) is negligible no longer holds. This motivates the need to develop 3D PBL parameterizations that include horizontal shear production of TKE. However, observational datasets that quantify the relative contributions of horizontal versus vertical shear production are still lacking. We deployed a combined measurement strategy utilizing small uncrewed aircraft systems (UAS) and Doppler wind lidar stations to provide the missing high-resolution measurements and thus to improve the understanding of multi-scale exchange processes in mountainous regions.
The measurement strategy incorporated commercially available and automatically operating multi-rotor UAS equipped with fast-response meteorological sensors to collect high-resolution measurements of the 3D wind vector, temperature and humidity, with additional aerosol particle measurements. During the TEAMx 2025 summer Extended Observation Period, four UAS performed simultaneous in-situ measurements at multiple heights and key valley locations (valley floor, foot of sidewall, mountain slope and crest) along a valley transect in the Inn Valley at the TEAMx Radfeld supersite in Austria. This included vertical profiles up to 2 km above mean sea level and horizontal cross-sections through the valley. The vertical profile spacing was representative of the grid resolution of targeted operational weather forecast simulations and was coordinated with the locations of the three deployed Doppler wind lidar systems, which continuously measured vertical profiles of wind.
The combined measurements deliver a unique observational dataset of wind distribution in the Inn Valley, enabling a spatially and temporally highly-resolved analysis of horizontal and vertical wind shear. The UAS measurement systems resolve the turbulent scales of wind up to 3 Hz, which corresponds to a vortex size of about 3 m at a mean horizontal wind speed of 10 ms-1, allowing the calculation of turbulent kinetic energy and turbulent fluxes. For up-valley winds, which are thermally driven and characteristic of the afternoon in mountain valleys, TKE increases in the horizontal direction from the valley center toward the mountain and reaches its vertical maximum near the mountain ridge. This observed rise in TKE coincides with strong horizontal wind shear, peaking at 0.01 s-1 near the mountain ridge, with the horizontal wind speed decreasing toward the mountain. By combining UAS- and lidar-based measurements with model parameterization development within the TEAMx framework, we aim to make turbulence representation in high-resolution numerical weather prediction models both more accurate and physically grounded, leading to more reliable forecasts in mountainous regions.

How to cite: Kippenberger, M., Schön, M., Ruhl, M., Wahl, E., Freddi, G., Gohm, A., Lehner, M., Bange, J., and Platis, A.: Measuring Horizontal Shear and Turbulence in Mountain Valleys using UAS and Lidar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20164, https://doi.org/10.5194/egusphere-egu26-20164, 2026.

EGU26-2998 | Orals | AS4.2

Mountain-wave influence on polar stratospheric ice clouds: evidence from MIPAS–ERA5 analysis 

Ling Zou, Reinhold Spang, Sabine Griessbach, Lars Hoffmann, Farahnaz Khosrawi, Rolf Müller, and Ines Tritscher

Mountain-wave-induced temperature perturbations can locally enable the formation of polar stratospheric clouds (PSCs). We examine a decade-long (2002–2012) record of ice PSCs derived from MIPAS/Envisat measurements. The points with the smallest temperature difference (ΔTice_min) between the frost point temperature (Tice) and the environmental temperature along the line of sight have been proposed and shown to provide a better estimate of the location of ice PSC observation from MIPAS. The temperature for the ice PSC observations is analyzed based on ERA5. Following this, we investigated the temperature history of the ice PSCs detected above Tice at the observation points along 24 h backward trajectories.

We find that 52 % of Arctic and 26 % of Antarctic ice PSCs are detected above Tice, with pronounced clustering over mountainous terrain and in downstream regions. The backward trajectories were calculated by using the MPTRAC model,  initialized at the ΔTice_min locations. Analysis of the temperature evolution along these trajectories shows that the fraction of ice PSCs at a temperature above Tice along the trajectory decreases, with the strongest decrease within the 6 h before observation. Accounting for temperature fluctuations along the air-mass histories, reduces the fractions of too warm ice PSCs at observation to 33 % in the Arctic and 9 % in the Antarctic.

These results demonstrate the substantial role of orographic waves in ice PSC formation and provide observational constraints for chemistry–climate model evaluation. This contribution is based on the published analysis of Zou et al. (2024, Atmos. Chem. Phys., 24, 11759–11774, https://doi.org/10.5194/acp-24-11759-2024) .

How to cite: Zou, L., Spang, R., Griessbach, S., Hoffmann, L., Khosrawi, F., Müller, R., and Tritscher, I.: Mountain-wave influence on polar stratospheric ice clouds: evidence from MIPAS–ERA5 analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2998, https://doi.org/10.5194/egusphere-egu26-2998, 2026.

EGU26-3966 | ECS | Orals | AS4.2

Climatology and trends of fog in the Svalbard region 

shubham singh and Moa K. Sporre

Fog is a common feature of the lower atmosphere in the Arctic, yet its long-term variability, seasonal changes, and sensitivity to rapid climate warming remain poorly known. Using meteorological data from five Svalbard stations from 1970 to 2020, we analyse seasonal fog occurrence, fog type (advection versus radiation), temperature, wind patterns. We also use sulphate aerosol data from one Svalbard station to investigate aerosol conditions.

High fog frequencies (7-15 %) are seen at the stations located on smaller islands in the vicinity of Svalbard (Janmayen, Bjørnøya, Hopen). The other two sites, located at Spitsbergen (Svalbard Airport, Ny-Ålesund), show substantially lower fog frequencies (0-4%). During summer, the fog frequency is highest for all stations, with radiation fog dominating at Spitsbergen sites while on the island stations, both advection fog and radiation fog is types are common. During winter, advection fog is predominant from cold, northerly to northeasterly marine airflows at most sites. The temperature during advection fog in winter is colder than during the formation of radiation fog. Spring and autumn seasonal represent transitional periods, with both fog types occurring but at lower overall frequencies. The wind direction during fog change seasonally, shifting from northerly/easterly in winter to southerly/westerly in summer.

Fog occurrence has decreased at most sites between 1970 and 2020. The drop is especially noticeable at Janmayen and Bjørnøya. The fog frequency at the Spitsbergen sites is also declining but with a weaker decreasing trend. The analysis shows that it is advection fog that is decreasing and not radiation fog. Regional warming, reduced sea-ice extent, and lower Arctic aerosol loading could be responsible for this decreasing trends. These results indicate that fog is sensitive to climate change in the Arctic. It changes visibility, the local radiation budget, and the way air and sea interact in an environment that is changing quickly.

How to cite: singh, S. and Sporre, M. K.: Climatology and trends of fog in the Svalbard region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3966, https://doi.org/10.5194/egusphere-egu26-3966, 2026.

EGU26-6771 | ECS | Orals | AS4.2

Spatial and temporal patterns of fog and low clouds in the Polar regions 

Olimpia Bruno and Jan Cermak

Low-level clouds and fog play a crucial role in the surface energy balance of polar regions, where even small perturbations in radiative fluxes can trigger amplified climatic responses. In these environments, the frequent presence of fog and stratiform low clouds strongly modulates both shortwave and longwave radiation, exerting a dominant control on near-surface temperature. The radiative effect of these clouds is highly sensitive to their thermodynamic phase: liquid-containing clouds generally enhance downwelling longwave radiation, promoting surface warming, whereas ice-dominated clouds are more transparent in the infrared and can contribute to surface cooling, particularly during polar night. As both the Arctic and Antarctic undergo rapid warming accompanied by shifts in cloud phase partitioning, understanding the occurrence and temporal variability of liquid and ice fog and low clouds is essential for accurately representing polar climate feedbacks and their role in ongoing climate change.

Using 11 years of cloud observations from the active satellite sensor CALIPSO, we characterize the spatial and temporal patterns of fog and low clouds (FLCs) across the polar regions, stratified by season and light conditions. Our results show a pronounced reduction in ice FLCs over Antarctica (~1% per year), while the Southern Ocean exhibits a decrease in liquid FLCs during winter under both daytime and nighttime conditions. In the Arctic, both liquid and ice FLCs decrease over land and sea-ice-covered regions from fall to spring. Over the Arctic Ocean, however, we find an increase in liquid FLCs during these seasons regardless of solar angle, whereas ice FLCs increase only under conditions of available solar radiation.

Overall, the observed trends in fog and low-level clouds suggest a potentially important role in modulating polar surface energy budgets.

How to cite: Bruno, O. and Cermak, J.: Spatial and temporal patterns of fog and low clouds in the Polar regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6771, https://doi.org/10.5194/egusphere-egu26-6771, 2026.

EGU26-7721 | Orals | AS4.2

Constraints on Southern Ocean Mesoscale Cellular Convective Cell Growth 

Anna Possner, Jessica Danker, Isabel McCoy, and Odran Sourdeval

Mesoscale cellular convection (MCC), which can be found in- and outside marine cold air outbreaks (MCAOs) over the Southern Ocean (SO), has been shown to influence the cloud radiative effect and potentially shortwave cloud feedbacks. While MCC morphology and cell-size scaling have been studied extensively in the subtropics and North Atlantic MCAOs, far less is known about how these relationships behave in the SO, where mixed-phase clouds dominate. In this study, we investigate the physical controls on MCC cell size and its variability during SO MCAOs based on collocated active and passive remote sensing products and reanalysis fields.

Specifically we combine MODIS retrievals of liquid water path and 0.86 μm reflectance for MCC classification and cell identification, ERA5 reanalysis for dynamical and thermodynamic fields, and DARDAR-v2 radar–lidar profiles to determine cloud-top height, cloud-top temperature, and cloud phase. Image segmentation applied to 200 × 200 km² scenes along DARDAR overpasses yields a catalogue of 19,500 MCC cells, 86% of which are supercooled—a clear reflection of the high prevalence of mixed-phase clouds in the SO.

Contrary to established behaviour in shallow NH boundary layers, we find no evidence of a constant aspect-ratio regime and no systematic deepening of the BL during MCAO evolution. Open and closed cells exhibit similar median diameters (~36–37 km), although open cells display a longer tail toward larger sizes. Thermodynamic and dynamic conditions—including stability parameter M, BL depth, and surface forcing—show minimal influence on cell-size variability. Approximately half of all mixed-phase open cells occur within MCAO regimes defined by M > –5 K, yet cell diameter remains largely insensitive to the strength of the outbreak.

Backward trajectory analysis indicates that time since cold air mass formation may play a more decisive role: larger cells tend to reside in older, more mature MCAO air masses. Our findings suggest that, in the SO, MCC cell growth is primarily constrained by air-mass age rather than boundary-layer deepening or thermodynamic forcing.

How to cite: Possner, A., Danker, J., McCoy, I., and Sourdeval, O.: Constraints on Southern Ocean Mesoscale Cellular Convective Cell Growth, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7721, https://doi.org/10.5194/egusphere-egu26-7721, 2026.

EGU26-10742 | ECS | Orals | AS4.2

How can EarthCARE satellite observations help improve Greenland’s clouds in the regional climate model RACMO? 

Thirza Feenstra, Willem Jan van den Berg, Gerd-Jan van Zadelhoff, David P. Donovan, Christiaan T. van Dalum, and Michiel R. van den Broeke

Clouds play an important role in Greenland’s surface mass balance, as they govern accumulation through precipitation and influence surface melt by altering the radiative balance. Therefore, correctly representing clouds in polar regional climate models is crucial for obtaining reliable surface mass balance estimates and projections. However, the complex, small-scale cloud microphysical processes involved in cloud formation, dissipation, and phase changes are often poorly represented in models. As in-situ observations of polar clouds are sparse, satellite observations can be an effective tool for evaluating and improving climate models. The new EarthCARE satellite, launched in May 2024, provides high-resolution co-located observations of the vertical structure of clouds and aerosols, and top-of-atmosphere radiation. Here, we show how these observations can be used to evaluate cloud representation in climate models by comparing them with output of the polar regional climate model RACMO (version 2.4p1).

We will present a comparison of over one year of multi-instrument EarthCARE observations of clouds and radiation for the Greenland region with model output that is co-located in time and space. We find that for clouds in all phases (solid, liquid, and mixed), RACMO tends to miss clouds at higher altitudes and underestimates water content for most locations and vertical levels. As a result, in RACMO, snowfall is less often generated at higher altitudes but more often at lower altitudes. However, the simulated snowfall rates are underestimated. Rainfall shows similar patterns, with rainfall modeled more frequently, but with lower rainfall rates. We will use these comparisons, along with EarthCARE’s radiation observations and retrieved cloud microphysical properties, to work towards improved cloud representation, surface radiation, and surface mass balance estimates in RACMO.

How to cite: Feenstra, T., van den Berg, W. J., van Zadelhoff, G.-J., Donovan, D. P., van Dalum, C. T., and van den Broeke, M. R.: How can EarthCARE satellite observations help improve Greenland’s clouds in the regional climate model RACMO?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10742, https://doi.org/10.5194/egusphere-egu26-10742, 2026.

EGU26-11006 | ECS | Posters on site | AS4.2

Quantifying drivers of the thermal-infrared radiative effect of Arctic low-level clouds in cold air outbreaks 

Sophie Rosenburg, Michael Schäfer, André Ehrlich, Anna Luebke, Marcus Klingebiel, Joshua Müller, and Manfred Wendisch

Marine cold air outbreaks (CAOs) represent an important meridional transport mechanism out of the Arctic towards lower latitudes. The cloud field properties change with the air mass transformation, and the thermal-infrared all-sky cloud radiative effect (CRE) is increasing in the downstream direction during the initial stages of a CAO. These evolution processes are important to understand current and future CAOs in a warming Arctic, which will favor weaker events.

Here, we aim to identify the driving factors of this downstream increase for different CAO events of varying intensity, which were observed during the HALO-(AC)3 campaign in spring 2022. The High Altitude and LOng range research aircraft (HALO) sampled CAOs in a quasi-Lagrangian way with a remote sensing payload. The thermal-infrared imager VELOX (Video airbornE Longwave Observations within siX channels) provided 2D broadband (7.7 µm to 12.0 µm) brightness temperature fields of cloud tops and the surface with a spatial resolution of 10 m for a 10 km target distance. First, a cloud mask is applied to those brightness temperature fields to determine cloud fractions. In a next step, two types of CRE are calculated. A cloud-only CRE is derived for all identified cloud pixels while an all-sky CRE is calculated for cloud-free as well as cloud pixels. The comparison of the cloud-only and all-sky VELOX CREs enables a determination of the all-sky CRE driver, i.e., cloud top temperature or cloud fraction. In addition, lidar cloud top heights and a large-scale all-sky CRE, based on measurements by a broadband radiometer and radiative transfer simulations, are analyzed to provide further context for the analyzed cases. The results imply that the strength of the all-sky CRE increase depends on the CAO intensity and is in general driven by increasing cloud fraction. Thus, this analysis provides a TOA-like perspective on the thermal-infrared radiative impact of a low-level cloud field, which is (trans-)forming during the initial stages of a CAO.

How to cite: Rosenburg, S., Schäfer, M., Ehrlich, A., Luebke, A., Klingebiel, M., Müller, J., and Wendisch, M.: Quantifying drivers of the thermal-infrared radiative effect of Arctic low-level clouds in cold air outbreaks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11006, https://doi.org/10.5194/egusphere-egu26-11006, 2026.

EGU26-12413 | ECS | Posters on site | AS4.2

Atmospheric transport characteristics during warm-air intrusions – focusing on aerosol, energy, and moisture transport 

Andreas Plach, Sabine Eckhardt, Nikolaos Evangeliou, and Annica M. L. Ekman

Arctic Amplification is not well understood. It is the result of a complicated interplay between remote and local forcing and feedback processes. Therefore, it is crucial to enhance our understanding of the transport of energy and moisture from lower latitudes. The amount of aerosol in the Arctic is also an important quantity as their role in Arctic Amplification, via direct radiative forcing and aerosol-cloud interactions, remain poorly quantified.

In this work, we aim to better quantify how aerosols, energy, and moisture are transported to and distributed within the Arctic. We investigate observations at Arctic stations, including, Villum and Zeppelin, and perform backward-in-time simulations with the Lagrangian atmospheric transport model FLEXPART (Pisso et al., 2019; Bakels et al., 2024) to derive so-called emission sensitivities and use these sensitivities to better quantify source regions of aerosols, energy, and moisture.

In general, we aim to better describe the spatial and temporal atmospheric transport characteristics into the Arctic and how these characteristics have changed in recent years. We focus on the transport during warm-air intrusions, since almost 30% of the total poleward transport of moisture (during winter) occurs during such events (Woods et al., 2013). Warm-air intrusions are often associated with large-scale atmospheric blocking patterns forcing a change in transport direction from east to more poleward, bringing warm, moist, and cloudy air into the Arctic. Warm-air intrusions can also be favourable for an enhanced transport of aerosols (e.g., Dada et al., 2022).

Since climate models show large biases in moisture flux during these events (Woods et al., 2017), there is clearly a need to better quantify the transport of moisture, energy, and aerosols during these events. This will also help to provide better forcing for climate simulations.

Bakels et al. (2024): 10.5194/gmd-17-7595-2024; Dada et al. (2022): 10.1038/s41467-022-32872-2; Lapere et al. (2024): 10.1029/2023JD039606; Pisso et al. (2019): 10.5194/gmd-12-4955-2019; Woods et al. (2013): 10.1002/grl.50912; Woods et al. (2017): 10.1175/JCLI-D-16-0710.1

How to cite: Plach, A., Eckhardt, S., Evangeliou, N., and Ekman, A. M. L.: Atmospheric transport characteristics during warm-air intrusions – focusing on aerosol, energy, and moisture transport, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12413, https://doi.org/10.5194/egusphere-egu26-12413, 2026.

EGU26-12546 | ECS | Orals | AS4.2

Quantifying the temporal variability of water vapor in Ny-Ålesund and its relation to weather systems 

Christian Buhren, Susanne Crewell, Claire Pettersen, Phillip Eisenhuth, Christoph Ritter, and Kerstin Ebell

The role of Water Vapor (WV) in Arctic amplification remains uncertain and is under investigation (Wendisch and coauthors, 2023). Understanding its role in the mechanisms driving Arctic amplification requires detailed information on its spatio-temporal variability. However, WV variability in the Arctic has rarely been examined. Temporally highly resolved integrated water vapor (IWV) data from ground-based MWR observations are ideally suited for the analysis of WV temporal variability. In this study, we make use of 13 years of measurements of the Humidity and Temperature PROfiler (HATPRO) at the AWIPEV atmospheric observatory (Ny-Ålesund, Svalbard). Extreme events of atmospheric moistening and drying are identified, characterized, and further related to the prevailing circulation weather systems. Since WV transport into the Arctic is episodic and primarily occurs through brief, intense events typically associated with cyclones (Henderson et al., 2021), it is essential to analyze these events in further detail. To analyze these events, we identify minima and maxima in the IWV time series. We define “extreme” using a threshold in IWV amplitudes within a respective time interval. An event can either consist of only one maximum (moistening) or minimum (drying) or of multiple maxima/minima.

When focusing on extreme atmospheric moistening and drying events, we find that absolute IWV amplitudes are highest in summer and lowest in winter. The events last between 2 and 142 hours. By contrast, winter shows a greater relative variability (with respect to the monthly mean) than summer, with IWV changes exceeding 250% within a few hours in some cases. Events with only one maximum (moistening) or one minimum (drying) are short-lived (75% last less than 24 hours), while those with multiple maxima/minima last longer, with a mean of 48 hours. We find that extreme atmospheric moistening and drying at Ny-Ålesund proceed differently: drying happens more rapidly but with smaller amplitudes than moistening. Also, the synoptic regimes favoring moistening and drying differ. For moistening the weather types ASW, AW, AS, and CSE account for half of the extreme moistening events, with the anticyclonic types transporting moisture over the North Atlantic. In contrast, CSE is associated with moisture transport over Scandinavia and West Russia, spanning the Barents and Kara Seas. For drying, significantly different weather systems can be responsible. Other studies found a positive trend in cyclone activity over the Barents Sea (e.g., Wickström et al., 2019), which could favor greater moisture transport driven by CSE.

We gratefully acknowledge the funding by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – Project Number 268020496 – TRR 172, within the framework of the Transregional Collaborative Research Center “ArctiC Amplification: Climate Relevant Atmospheric and SurfaCe Processes, and Feedback Mechanisms (AC)³”.  We thank the AWIPEV team for their support in operating our instruments at AWIPEV within the project AWIPEV_0016.

How to cite: Buhren, C., Crewell, S., Pettersen, C., Eisenhuth, P., Ritter, C., and Ebell, K.: Quantifying the temporal variability of water vapor in Ny-Ålesund and its relation to weather systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12546, https://doi.org/10.5194/egusphere-egu26-12546, 2026.

EGU26-14343 | ECS | Posters on site | AS4.2

New insights into Arctic mixed-phase clouds from airborne and EarthCARE observations 

Lars van Gelder, Pavlos Kollias, Mario Mech, Lukas Pfitzenmaier, and Susanne Crewell

Low-level Arctic clouds, especially mixed-phase clouds, are key drivers of regional climate and Arctic amplification, yet their microphysical and dynamical properties remain difficult to observe in data-sparse regions. EarthCARE offers new opportunities to address this observational gap; however, its measurements require validation using independent reference data. As a contribution to these validation activities, the Polar 5 research aircraft of the Alfred Wegener Institute has been equipped with an EarthCARE-like instrument suite and operated during the COMPEX-EC (Clouds over cOMPlEX environment – EarthCARE) in April 2025 from Kiruna, Sweden. During seven research flights, we collected more than 5 hours of along-track airborne radar measurements collocated with EarthCARE overpasses, covering diverse Arctic conditions from marine cold-air outbreaks (CAO) over the Norwegian Sea to cloud fields over northern Scandinavia. For moving platforms, such as aircraft, corrections addressing horizontal and vertical motion, as well as attitude, need to be applied to some of the measurements. Hereby, the Doppler velocity is especially challenging, and this is further complicated by the installation of the W-band Microwave Radar/radiometer for Arctic Clouds (MiRAC) on Polar 5 in a belly pod with a 25° inclination under the aircraft, which enhances the complexity. MiRAC is complemented by a microwave radiometer, an Airborne Mobile Aerosol Lidar for Arctic research (AMALi), spectral and broadband radiative sensors, and dropsondes. The collected data provide a unique basis for evaluating EarthCARE cloud products, with a particular focus on cloud geometric properties and vertical cloud structure. Cloud-top heights are derived from AMALi and MiRAC and compared to spaceborne retrievals from EarthCARE ATLID and CPR across different Arctic cloud regimes. We exploit the complementary sensitivities of lidar and radar to assess the detectability of thin liquid-topped clouds and mixed-phase cloud layers. Dropsondes released during EarthCARE overpasses provide thermodynamic and wind profiles that support the interpretation of observed cloud structures and precipitation occurrence. Beyond EarthCARE validation, the dataset contributes to an enhanced understanding of Arctic cloud vertical structure and its relevance to precipitation development under different synoptic conditions. Ongoing work aims to extend the analysis towards Doppler-based interpretations of cloud dynamics.

This work was supported by the DFG funded Transregio-project TRR 172 "Arctic Amplification (AC)³".

How to cite: van Gelder, L., Kollias, P., Mech, M., Pfitzenmaier, L., and Crewell, S.: New insights into Arctic mixed-phase clouds from airborne and EarthCARE observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14343, https://doi.org/10.5194/egusphere-egu26-14343, 2026.

EGU26-14797 | Posters on site | AS4.2

Toward enhanced retrievals of supercooled droplet properties in Antarctic clouds  

Martin Radenz, Michael Lonardi, Yolanda Temel, Teresa Vogl, Ronny Engelmann, Julia Schmale, and Patric Seifert

Clouds containing supercooled liquid are common over the Southern Ocean and coastal Antarctica. The liquid phase not only has strong influence on the surface energy budget, but also cloud microphysics and precipitation formation. Often, the droplets occur in thin layers stacked on top of each other and/or coexisting with ice particles. Both of these aspects pose a significant challenge for observations. Cloud radar Doppler spectra can contain this information in the form of individual peaks for different particle populations, but extracting useful data is challenging for automated retrievals.

Combining advanced Doppler spectra analysis techniques with established retrieval methods, such as ACTRIS-Cloudnet, can provide cloud microphysical properties even under complex conditions. This approach has been applied to observations from Neumayer Station III, Antarctica (70.67°S, 8.27°W), where synergistic remote sensing instruments are operated since 2023. During the 2024/25 austral summer, tethered-balloon in-situ observations provided complementary information on cloud droplet properties.

Two aspects will be presented: Firstly, properties of liquid layers in geometrically thick snowfall clouds. Spatiotemporal coinciding balloon-borne observations provide independent verification. Secondly, observations of seeder-feeder situations, in which ice crystals sediment into a supercooled – potentially drizzling – layer. It is envisaged that the Doppler spectral analysis will be implemented as a new method in ACTRIS-Cloudnet in the future.

How to cite: Radenz, M., Lonardi, M., Temel, Y., Vogl, T., Engelmann, R., Schmale, J., and Seifert, P.: Toward enhanced retrievals of supercooled droplet properties in Antarctic clouds , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14797, https://doi.org/10.5194/egusphere-egu26-14797, 2026.

EGU26-14927 | Posters on site | AS4.2

Unpacking Global Drivers of Extreme Precipitation over West Antarctica, using a Variable-Resolution Earth Systems Model with Explicit Moisture Tagging 

Rajashree Datta, Adam Herrington, Jesse Nusbaumer, and Luke Trusel

The overall gain and loss of snow and ice on the surface of the Antarctic ice sheet is strongly driven by rare extreme events, some of which result from atmospheric rivers transporting both moisture and heat from the tropics towards the south pole. Moisture transport is strongly driven by large-scale patterns, e.g. the El Niño Southern Oscillation, the Southern Annular Mode, PSA1 and PSA2 patterns. Additionally, in recent years, the Southern Ocean region has witnessed major changes, including sequential record lows for sea ice extent and warming oceans, with direct impacts on the Antarctic ice sheet and Southern Ocean. Previous research has highlighted the strong sensitivity of precipitation in West Antarctica to large-scale patterns, and especially the importance of atmospheric rivers. However, atmospheric rivers are only one mechanism of transport, and estimates are subject to the reliability of detection algorithms. Additionally, the ability to fully-capture drivers and impacts of extreme events are limited by spatiotemporal resolution in Earth Systems Models.

Here, we employ a variable-resolution version of the global Community Earth Systems Model (VR-CESM2) with enhanced resolution over Antarctica over the historical period (1990-2020), run at a high time-resolution capable of capturing extremes and calculating atmospheric rivers. We additionally employ moisture-tagging (linking precipitation to a moisture source region), which can quantify links between sources and sinks of extreme precipitation directly and identify mechanisms which drive transport. Here, we will focus on drivers of extremes in West Antarctica, comparing mechanisms identified via direct moisture tagging with those concurrent with atmospheric rivers.

 

How to cite: Datta, R., Herrington, A., Nusbaumer, J., and Trusel, L.: Unpacking Global Drivers of Extreme Precipitation over West Antarctica, using a Variable-Resolution Earth Systems Model with Explicit Moisture Tagging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14927, https://doi.org/10.5194/egusphere-egu26-14927, 2026.

EGU26-15936 | ECS | Orals | AS4.2 | Highlight

Observed cloud and atmospheric drivers of surface radiation change 2001-2023 on the North Slope of Alaska 

Leah Bertrand, Jennifer Kay, and Gijs de Boer

Arctic surface warming is driven by a changing surface energy budget. However, sparse observations in the Arctic limit our ability to identify drivers of surface energy budget change. Here, we leverage detailed long-term observations at the Atmospheric Radiation Measurement (ARM) program's North Slope of Alaska (NSA) facility to constrain and attribute drivers of surface radiation change 2001-2023. We combine cloud and atmospheric observations with radiative transfer calculations, allowing us to quantify the relative impact of clouds, temperature, and water vapor on surface radiation trends and variability. At the ARM NSA facility, downwelling longwave radiation is increasing year-round and downwelling shortwave radiation is decreasing during summer. We find that cloud changes intensify the downwelling longwave radiation trend, which is largely due to warming. We also find that cloud changes drive decreasing downwelling shortwave radiation during summer. These results reveal the important role of clouds in driving surface radiation trends along the North Slope of Alaska.

How to cite: Bertrand, L., Kay, J., and de Boer, G.: Observed cloud and atmospheric drivers of surface radiation change 2001-2023 on the North Slope of Alaska, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15936, https://doi.org/10.5194/egusphere-egu26-15936, 2026.

EGU26-16990 | ECS | Posters on site | AS4.2

Model analysis of convective precipitation in the Arctic 

Sophie Vliegen and Johannes Quaas

The strong warming of the Arctic has profound implications for the atmospheric energy budget. Recent studies indicate that the Arctic energy balance is transitioning from a predominantly radiative-advective equilibrium towards a radiative-advective convective regime.

Using monthly CMIP6 model output from an idealized CO2-forcing scenario, we analyze changes in the occurrence of convective precipitation relative to total precipitation. Our results show a pronounced seasonal and surface-dependent signal. This pattern is also reflected in the associated trend estimates. However, the inter-model spread across the CMIP6 models is substantial, with individual models even exhibiting opposing trend signs. This large spread is consistent with pronounced differences in simulated sea ice extent among the models, suggesting potential linkages to other key variables.

How to cite: Vliegen, S. and Quaas, J.: Model analysis of convective precipitation in the Arctic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16990, https://doi.org/10.5194/egusphere-egu26-16990, 2026.

EGU26-17535 | ECS | Posters on site | AS4.2

Cloud state transitions at Ny-Ålesund: A machine learning supported statistical analysis 

Andreas Walbröl, Nils Risse, Dwaipayan Chatterjee, Susanne Crewell, and Kerstin Ebell

Clouds are still a major source of uncertainty in projections of the future climate because of complex feedback mechanisms and their interplay with other atmospheric and surface properties (i.e., through solar and thermal-infrared radiation and precipitation). In the Arctic, where the climate is projected to warm the strongest, clouds pose a particular challenge to current climate and weather forecast models because of the difficulties in simulating the frequently occurring mixed-phase clouds and the sparsity of observational data.

In this study, we aim to improve our understanding of Arctic clouds on multi-annual time scales by performing statistical analyses of cloud states and their transitions using cloud radar data from the research site Ny-Ålesund, Svalbard. We have gathered nine years of comprehensive cloud and precipitation observations with the 94-GHz cloud radars, which were operated at the German-French Arctic Research Base AWIPEV observatory in synthesis with other in-situ and remote sensing instruments (i.e., microwave radiometers, lidar, disdrometers, ...). The additional meteorological measurements also allow us to study how atmospheric conditions affect the cloud states and transitions.

Modern machine learning algorithms are well suited to analyse big data sets and reveal features imperceptible to the human eye because of the complexity of the problem. We train a Vision Transformer [1-3] with height-resolved cloud radar reflectivities, Doppler velocities, ceilometer data and liquid water path-sensitive brightness temperatures at 89 GHz in a self-supervised framework. The Vision Transformer learns to identify distinct features in the training data and therefore find different cloud states without direct human intervention.

Here, we present our first steps focussing on the interpretation of the machine learning model output and fine tune the settings to better discern the cloud states. Different cloud macro- and microphysical properties are tested to understand the nature of each cluster the machine learning algorithm produced.

Later, we will apply the trained machine learning algorithm to synthetic radar data simulated with the Passive and Active Microwave radiative TRAnsfer (PAMTRA, [4]) model based on the output of the ICOsahedral Non-hydrostatic (ICON, [5]) model in large-eddy configuration. By comparing the observation-based analysis with the one performed on the simulated radar data we aim to further shed light on the strengths and weaknesses of ICON regarding cloud states and transitions.

 

We gratefully acknowledge the funding by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) - Project Number 268020496 - TRR 172, within the framework of the Transregional Collaborative Research Center "ArctiC Amplification: Climate Relevant Atmospheric and Surface Processes, and Feedback Mechanisms (AC)³". We also acknowledge the support of AWIPEV for the project AWIPEV_0016.

[1]: Vaswani, A., et al., 2017, Inc. arXiv, 1706.03762, https://arxiv.org/abs/1706.03762.

[2]: Caron, M., et al., 2021, arXiv, 2104.14294, https://arxiv.org/abs/2104.14294.

[3]: Chatterjee, D., et al., 2024, Geophys. Res. Lett., 51, 12, e2024GL108889, doi: 10.1029/2024GL108889.

[4]: Mech, M. et al., 2020, Geosci. Model Dev., 13, 4229-4251, doi: 10.5194/gmd-13-4229-2020.

[5]: Zängl, G. et al., 2015, Q. J. R. Meteorolog. Soc., 141, 563-579, doi: 10.1002/qj.2378.

 

How to cite: Walbröl, A., Risse, N., Chatterjee, D., Crewell, S., and Ebell, K.: Cloud state transitions at Ny-Ålesund: A machine learning supported statistical analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17535, https://doi.org/10.5194/egusphere-egu26-17535, 2026.

EGU26-17911 | Posters on site | AS4.2

A decade beneath Arctic clouds: Continuous radar observations at Ny-Ålesund, Svalbard 

Kerstin Ebell, Mario Mech, Andreas Walbröl, Christian Buhren, Pavel Krobot, Christoph Ritter, and Marion Maturilli

Climate change signals are especially strong in the Arctic, where warming from 1979 to 2021 proceeded at nearly four times the global average rate (Rantanen et al., 2022). The magnitude of this warming varies across the region, and the Svalbard archipelago, located in the warmest part of the Arctic, has experienced particularly intense temperature increases (Dahlke and Maturilli, 2017).

The influence of clouds on the rapidly evolving Arctic climate system, as well as the processes governing their behavior, remains a key research challenge. Although detailed cloud observations are essential, only a limited number of Arctic sites provide continuous, high-resolution vertical measurements of cloud properties. One such site is the German-French Arctic Research Base AWIPEV at the Ny-Ålesund Research Station on Svalbard. Since 2016, a 94 GHz cloud radar has been operating at this location as part of the Transregional Collaborative Research Centre TR172 on Arctic Amplification (AC)³ (http://www.ac3-tr.de; Wendisch et al., 2023). In combination with complementary remote-sensing instruments, including ceilometers and microwave radiometers, this observational setup allows for continuous cloud monitoring with high temporal and vertical resolution. This presentation highlights key results derived from a decade of cloud radar observations.

Clouds are present at Ny-Ålesund during roughly 78% of the time, most frequently at low levels between 0.5 and 1.5 km. While pure liquid clouds show a distinct seasonal variability, mixed-phase clouds occur year-round and account for about 42% of all cloud observations. These liquid-containing clouds have a significant influence on the Arctic surface energy budget, leading to an overall warming at Ny-Ålesund due to the enhanced longwave downward radiation flux.

Based on the 10-year-long dataset, we will examine the interannual variability of clouds and precipitation at Ny-Ålesund, as well as their impact on surface radiation.

Acknowledgment: We gratefully acknowledge the funding by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – Project Number 268020496 – TRR 172, within the framework of the Transregional Collaborative Research Center “ArctiC Amplification: Climate Relevant Atmospheric and SurfaCe Processes, and Feedback Mechanisms (AC)³”. We also acknowledge the support of AWIPEV for the project AWIPEV_0016.

How to cite: Ebell, K., Mech, M., Walbröl, A., Buhren, C., Krobot, P., Ritter, C., and Maturilli, M.: A decade beneath Arctic clouds: Continuous radar observations at Ny-Ålesund, Svalbard, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17911, https://doi.org/10.5194/egusphere-egu26-17911, 2026.

EGU26-18004 | ECS | Orals | AS4.2

Quantifying the Evolution of Cloud Street Structures During Arctic Marine Cold Air Outbreaks Using Satellite Observations 

Hannah Sundermann, Marcus Klingebiel, André Ehrlich, and Hartwig Deneke

The clouds associated with Marine Cold Air Outbreaks (MCAOs) exhibit characteristic structures, initially forming as roll clouds or cloud streets parallel to the wind direction, and eventually breaking up into a cellular cloud field.

Here, a novel correlation-based metric, the Correlation clOud Street Index (COSI) is introduced. It is defined as the Pearson correlation coefficient between an image and an optimally oriented and scaled Gabor kernel, providing a quantitative measure of cloud street presence and distinctness. The calculation of this index also extracts cloud street spacing (wavelength) and orientation as structural properties.

Applied to satellite observations with extensive spatial and temporal coverage, we utilise the COSI to get novel insights into the spatio-temporal evolution of cloud street structures in marine cold air outbreaks. By analysing sequences of consecutive satellite images for individual events, we capture the cloud evolution for both the overall MCAO and along quasi-Lagrangian trajectories. We quantify the systematic increase in cloud street wavelength with increasing distance from the ice edge and assess the aspect ratio (wavelength divided by cloud top height) across a larger dataset. The dependence on the MCAO strength is also evaluated. The cases analysed correspond to periods with (AC)3 aircraft campaigns, allowing the aircraft observations to be placed in a broader context and providing more detailed observations of meteorological conditions along flight trajectories.

This work was supported by the DFG funded Transregio-project TRR 172 “Arctic Amplification (AC)3“.

How to cite: Sundermann, H., Klingebiel, M., Ehrlich, A., and Deneke, H.: Quantifying the Evolution of Cloud Street Structures During Arctic Marine Cold Air Outbreaks Using Satellite Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18004, https://doi.org/10.5194/egusphere-egu26-18004, 2026.

EGU26-18430 | ECS | Posters on site | AS4.2

Exploring Aerosol-Cloud Interactions in Arctic Mixed-Phase Clouds Using ICON-LEM 

Lena Bruder, Christoph Ritter, Naruki Hiranuma, Hyojin Kang, and Vera Schemann

The contribution of Arctic mixed-phase clouds (MPCs) to the accelerated climate warming in the Arctic, known as Arctic amplification, remains uncertain due to complex microphysical and environmental interactions. Cloud condensation nuclei (CCN) concentrations influence MPC properties; however, current models often prescribe CCN levels much higher than Arctic observations suggest. To address this, we investigate the sensitivity of MPC properties to CCN concentrations using 600-m ICON-LEM simulations around Ny-Ålesund. The CCN sensitivity studies are based on typical CCN concentrations observed at the Zeppelin Observatory, serving as a benchmark for Ny-Ålesund conditions. We select simulation days by analyzing aerosol optical depth (AOD) measurements in Ny-Ålesund to represent high and low aerosol loading regimes, which are confirmed by Micro-Pulse Lidar (MPL) observations. Our initial studies, spanning mimicked Arctic, maritime, and polluted CCN regimes, reveal clear CCN effects: lower CCN concentrations reduce liquid water path (LWP) and increase radar reflectivity (Ze), mainly due to enhanced rain and graupel formation. However, the model underestimates the observed Ze, indicating shortcomings in the representation of phase partitioning. The results suggest that microphysical sensitivity varies with cloud height, with low-level MPCs responding more strongly than higher layers. We further explore this by separating cloud layers relative to the melting layer and analyzing their CCN sensitivity. To increase robustness, additional summer and winter low-level MPC cases are included. Complementing CCN sensitivity, ice nucleating particle (INP) sensitivity studies constrained by observed INP concentrations from the Gruvebadet observatory assess INP influence on phase-partitioning and precipitation in low-level MPCs. Identifying suitable CCN–INP combinations may improve MPC representation in ICON-LEM and deepen understanding of the aerosol-cloud interactions driving Arctic amplification.

This work was supported by the DFG-funded Transregio-project TRR 172 ”Arctic Amplification (AC)³”.

How to cite: Bruder, L., Ritter, C., Hiranuma, N., Kang, H., and Schemann, V.: Exploring Aerosol-Cloud Interactions in Arctic Mixed-Phase Clouds Using ICON-LEM, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18430, https://doi.org/10.5194/egusphere-egu26-18430, 2026.

EGU26-19611 | ECS | Orals | AS4.2

Precipitation processes in an Antarctic moist air intrusion: insights from multi-frequency radar observations over a 1100-km transect 

Heather Corden, Julien Delanoë, Felipe Toledo Bittner, and Alexis Berne

The ERC Synergy funded project AWACA aims to understand the atmospheric branch of the water cycle over Antarctica. It relies on innovative observations of the tropospheric meteorological conditions and the isotopic composition of water vapor and hydrometeors along a 1100-km transect between Dumont d’Urville station at the coast and Concordia station on the high inner Antarctic plateau. The deployment of instruments was completed in the austral summer season from November 2024 to February 2025. The instruments will remain in place for three years. At four locations along the transect, temporary container-stations were deployed. Each container includes, among other instruments, a Metek MIRA 35 GHz cloud radar, an MRR-PRO 24 GHz precipitation radar, and a BASTA 95 GHz cloud radar. Adjacent to each container is a comprehensive surface weather station.

This contribution will present a case study of a coastal cyclone and resulting moist air intrusion in February 2025, focusing on the radar data. Trajectory analysis confirmed that air parcels within the same intrusion traveled inland over multiple sites of the observational transect. However, the mechanisms by which the moisture of the intrusion is converted into precipitation differ between the coast and the high plateau. Taking advantage of the multi-frequency, spectral, polarimetric radar dataset, differences in the microphysics of snowfall along the transect have been investigated. On the coastal slope of the ice sheet, uplift, turbulence and the presence of liquid water lead to riming and aggregation of snowflakes. On the high plateau, dry and cold conditions lead to smaller snow particles, for which the variation in the radar signal appears to arise from variations in primary production and ice crystal habit.

How to cite: Corden, H., Delanoë, J., Toledo Bittner, F., and Berne, A.: Precipitation processes in an Antarctic moist air intrusion: insights from multi-frequency radar observations over a 1100-km transect, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19611, https://doi.org/10.5194/egusphere-egu26-19611, 2026.

EGU26-22022 | ECS | Posters on site | AS4.2

Assessing the Influence of Microphysics Parameterizations on In-Cloud Ground Icing Using WRF V 4.4  

Pravin Punde, Yngve Birkelund, and Trude Eidhammer

The precise simulation of in-cloud icing is essential for various atmospheric and aviation-related applications. This study aims to investigate the sensitivity of different microphysics schemes within the Weather Research and Forecasting model (WRF) V 4.4 in simulating in-cloud ground icing events during the period from May 2023 to April 2024 over Fagernes Mountain, a complex terrain site in northern Norway. Specifically, we will investigate the Thompson, Thompson-Eidhammer, WDM7, and P3 schemes. Microphysics schemes are critical in representing the formation, growth, and fallout of hydrometeors, within clouds, thereby significantly impacting the accuracy of cloud and precipitation forecasts in numerical weather prediction models.

Preliminary insights suggest that there may be significant variations in the simulation of in-cloud icing among the different microphysics schemes. For instance, one of our case studies has indicated that the Thompson scheme might excel at low icing rates, while the Morrison scheme could perform better at high icing rates. The Thompson-Eidhammer and P3 schemes are sophisticated and may provide more nuanced predictions of cloud liquid water and icing severity across various conditions. In contrast, simplerschemes might underestimate or overestimate icing conditions due to their less comprehensive treatment of microphysical processes. This study will highlight the importance of selecting an appropriate microphysics scheme based on specific meteorological conditions and the desired level of detail in the simulation. The results will underscore the need for continued refinement of microphysics parameterizations in numerical weather prediction models to improve the accuracy of in-cloud ground icing forecasts and other related applications.

How to cite: Punde, P., Birkelund, Y., and Eidhammer, T.: Assessing the Influence of Microphysics Parameterizations on In-Cloud Ground Icing Using WRF V 4.4 , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22022, https://doi.org/10.5194/egusphere-egu26-22022, 2026.

EGU26-192 | ECS | PICO | AS3.5

Evaluation of WRF-Chem aeolian dust emission and land surface models over the dust belt. 

Semontee Deb, Elena Louca, Angelos Violaris, Pantelis Kiriakidis, Yannis Proestos, and Theodoros Christoudias


Aeolian dust is a key component of the Earth system, influencing biogeochemical cycle, cloud microphysics, and the radiative energy budget and atmospheric dynamics, while also degrading air quality around major source regions. Large uncertainties persist in simulating atmospheric dust emission and transport, arising from the complex coupling between surface properties, boundary-layer processes, and atmospheric forcing. 

Previous efforts to evaluate the dust modelling performance of the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) have mostly relied on short-term or region-specific case studies, typically focused on individual dust outbreaks or restricted geographical domains.
In this study, we present a comprehensive, year-long evaluation of WRF-Chem (v4.7.1) over the dust belt spanning North Africa, the Middle East, and Central Asia. We evaluate an ensemble of six simulations using three widely applied dust emission schemes (GOCART, AFWA, and UoC) combined with two advanced land surface models (LSM): Noah-MP and CLM4. The ensemble model output is assessed against multiple observation and reanalysis datasets, including AERONET aerosol optical depth (AOD), the MODIS-derived MIDAS dust optical depth product, and ERA5-Land surface fields of soil moisture and wind speed, which control dust emission fluxes. 

Our analysis shows that land-surface representation exerts a strong influence on dust emission magnitude and spatial distribution, with Noah-MP yielding systematically higher agreement with observed meteorology and AOD. Among the dust emission schemes, AFWA performs most consistently, while UoC04 exhibits lower precision. Empirical scaling factors are derived for each dust emissions–LSM pairing.To our knowledge this is the first year-round, multi-scheme assessment of WRF-Chem dust performance, offering guidance for improved dust forecasting and climate applications. 

 

How to cite: Deb, S., Louca, E., Violaris, A., Kiriakidis, P., Proestos, Y., and Christoudias, T.: Evaluation of WRF-Chem aeolian dust emission and land surface models over the dust belt., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-192, https://doi.org/10.5194/egusphere-egu26-192, 2026.

Aerosols over the Indian region exhibi large spatial and seasonal Variation, however long-term ground-based Measurements that can consistently illustrate these variations are still limited. In this work, I utilize Level-2 AERONET data from selected locations in India to investigate how aerosol loading and optical attributes have changed during the last decade. The analysis centers chiefly on on Aerosol Optical Depth (AOD), Ångström exponent, and basic inversion products that help identify the dominant aerosol types.

The results indicate a clear seasonal variation at all stations. High AOD values appear during the pre-monsoon months, which is consistent with dust-laden air mass intrusion from arid regions, while winter months present increased fine-mode aerosols linked to vegetation fires and area-specific emission activities. Stations located in the Indo-Gangetic Plain exhibit the highest overall AOD levels, whereas coastal and semi-arid stations demonstrate lower values and more mixed aerosol regimes. Some sites indicate a gradual rise in fine-mode aerosol contribution, suggesting increasing anthropogenic influence, while others show small or no long-term trends.

These observations assist into better understand the aerosol environment over India and also furnish a reliable reference for measuring satellite retrievals. The study highlights how AERONET measurements can support regional climate and air-quality assessments by offering consistent, long-term optical property data that cannot be captured fully by satellites alone.

How to cite: Saxena, A.: Aerosol Characteristics over India Based on Long-Term AERONET Measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-261, https://doi.org/10.5194/egusphere-egu26-261, 2026.

EGU26-943 | ECS | PICO | AS3.5

UAV observations to reveal new insights into dust particle morphology and orientation 

Kenneth M. Tschorn, Konrad Kandler, Frank Gunther Wienhold, Maria Kezoudi, Alkistis Papetta, Kostas Fragkos, Kilian Schneiders, Zuhir Bona, and Franco Marenco

Atmospheric dust affects the Earth’s radiation budget through scattering and absorption, processes governed by its optical properties linked to their microphysical characteristics (size, shape, refractive index, and orientation). While knowledge of dust particle size has progressed in the last few decades, dust morphology remains poorly constrained beyond the generic category of “irregular particles”. Although some studies suggest that dust particles can exhibit preferred orientations within the atmospheric column, most radiative-transfer models still represent dust as ensembles of randomly oriented spheres or spheroids. The limited availability of direct observational evidence limits our understanding of how dust’s non-sphericity and orientation influence remote-sensing retrievals, atmospheric processes, and aerosol radiative forcing. Given that mineral dust accounts for one of the largest global mass fluxes of primary aerosols, reducing these uncertainties is crucial to better constrain its overall radiative impact.

 

To address these gaps, we collect new UAV-based datasets on dust particle shape, internal structure, and orientation. In spring 2025, the Cyprus Institute conducted a two-month UAV campaign aiming for two goals: (1) to advance airborne dust-sampling methods, and (2) to investigate dust composition, size, shape, and orientation. Multiple UAV platforms were deployed during eight dust-affected flight days, guided by daily dust and weather forecasts. This strategy enabled sampling of diverse atmospheric conditions, including a strong dust event on 17/05/2025 with total AOD at 500- nm approaching the value of 1. Additional campaigns will further expand the dataset.

 

The UAV payloads included the Compact Optical Backscatter Aerosol Detector (COBALD) and Giant Particle Collectors (GPAC), supplemented by Optical Particle Counters (OPCs). To detect signatures of particle orientation two COBALD instruments, each operating at two wavelengths (455 and 940 nm), were deployed in a dual-field-of-view configuration pointing horizontally and vertically with two nearly orthogonal viewing directions. GPAC were adapted to carry TEM grids (small, ultra-thin mesh substrates used to collect particles for transmission electron microscopy) enabling airborne dust sampling suitable for high-resolution imaging and 3-D reconstruction of particle morphology. These combined measurements provided a unique dataset for assessing dust particle morphology, size, and potential orientation effects in the atmospheric column.

How to cite: Tschorn, K. M., Kandler, K., Wienhold, F. G., Kezoudi, M., Papetta, A., Fragkos, K., Schneiders, K., Bona, Z., and Marenco, F.: UAV observations to reveal new insights into dust particle morphology and orientation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-943, https://doi.org/10.5194/egusphere-egu26-943, 2026.

EGU26-2760 | PICO | AS3.5

Tracing a Northern African Contribution to European Dust During the Last Glacial Maximum 

Denis-Didier Rousseau, Catherine Chauvel, Peter O Hopcroft, Pamela Gutiérrez, Ségolène Saulnier-Copard, Pierre Antoine, Markus Fuchs, and Alicja Ustrzycka

During the Last Glacial Maximum (LGM), global surface air temperatures were up to 6 °C lower than pre-industrial levels, and the mineral dust cycle intensified significantly, with global dust loading two to four times higher than during the Holocene. Loess deposits and Greenland ice cores record peak dust concentrations during this period. While Asian sources were traditionally considered the primary contributors to dust in Greenland, recent geochemical evidence indicates a mixture of Asian, North African, and European origins. Europe itself experienced heightened dust activity, predominantly attributed to local sources. Here, we present trace element data and Sr and Pb isotopic signatures from LGM-aged samples across 15 European sites, from a Western France to Ukraine longitudinal transect, revealing a notable contribution of fine dust from remote sources, particularly Northern Africa. These geochemical findings are corroborated by Earth System model simulations, which underscore Northern Africa's substantial role in dust deposition across the Northern Hemisphere during glacial periods.

Reference: Rousseau et al. (2025). A remote input of African dust to Last Glacial Europe. Comm. Earth & Environ., 6, 847. https://doi.org/10.1038/s43247-025-02888-9

How to cite: Rousseau, D.-D., Chauvel, C., Hopcroft, P. O., Gutiérrez, P., Saulnier-Copard, S., Antoine, P., Fuchs, M., and Ustrzycka, A.: Tracing a Northern African Contribution to European Dust During the Last Glacial Maximum, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2760, https://doi.org/10.5194/egusphere-egu26-2760, 2026.

EGU26-3373 | ECS | PICO | AS3.5

New processes to counteract sedimentation of coarse dust particles are required for climate models to agree with observations 

Natalie Ratcliffe, Claire Ryder, Nicolas Bellouin, Martina Klose, Stephanie Woodward, Anthony Jones, Ben Johnson, Lisa-Maria Wieland, Andreas Baer, Josef Gasteiger, and Bernadett Weinzierl

Recent observations show that large mineral dust particles are more abundant in the atmosphere than expected and travel further than their mass and theoretical rapid deposition allow for. The presence of these large particles alters the impact of dust on Earth’s radiative budget, carbon and hydrological cycles, and human health. Research into the impacts of the mechanisms influencing large dust particle lifetime in models is vital in ascertaining how large dust particles travel thousands of kilometres further than expected. We employ a series of model simulations to better understand the long-range transport of large particles from the Sahara to the West Atlantic. We present results from two models—HadGEM3A and ICON-ART—which are run at differing resolutions and with different dust representations (size bins and lognormal modes). Observations are used to verify long-range transport in model simulations, including in-situ aircraft observations at the Sahara, Canary Islands, Cape Verde, and Caribbean. Coarse particle mass loading (validated against observations) is limited by excessively rapid deposition in both models, but is further limited in ICON-ART by a reduced size-range representation, with the coarsest mode having a mean diameter by mass of 14.2 µm, whereas the maximum dust size in HadGEM3A extends to 63.2 µm. The sensitivity of large particle long-range transport to sedimentation, convective and turbulent mixing, shortwave absorption, and impaction scavenging are tested in global HadGEM3A climate simulations. A reduction in sedimentation by 80% is required to bring the modelled large particle transport into agreement with aircraft observations. None of the other processes tested were able to make the multiple order of magnitude changes to long-range large particle concentration in the model required for agreement with the observations. Convective and turbulent mixing in the model have minimal impact on large particle long-range transport, but are key in controlling the vertical distribution in the Saharan air layer and marine boundary layer, respectively. This work adds to the growing body of evidence that points to processes involved in large mineral dust transport and deposition which are not represented accurately or at all in models, which counteract the sedimentation of large particles in the real-world.

How to cite: Ratcliffe, N., Ryder, C., Bellouin, N., Klose, M., Woodward, S., Jones, A., Johnson, B., Wieland, L.-M., Baer, A., Gasteiger, J., and Weinzierl, B.: New processes to counteract sedimentation of coarse dust particles are required for climate models to agree with observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3373, https://doi.org/10.5194/egusphere-egu26-3373, 2026.

EGU26-3933 | ECS | PICO | AS3.5

Seasonal variability of mineral dust composition on an alpine snowpack in the Tateyama Mountains, Japan  

Pia Ataka, Ryo Sugiyama, Noboru Furukawa, and Nozomu Takeuchi

 Mineral dust deposited on snow surfaces plays an important role in snow and ice melting by reducing surface albedo and modifying surface energy balance. In addition to its direct radiative effects, mineral dust can indirectly enhance snow surface darkening by supplying nutrients that stimulate snow algal activity. Despite its importance, the sources and mineralogical characteristics of dust preserved in alpine snowpacks remain insufficiently constrained, particularly with respect to seasonal changes during the melt period.

 Most previous studies have interpreted mineral dust on snow as long-range transported material originating from continental desert regions. In alpine environments, however, progressive snow retreat during the melt season exposes surrounding ground surfaces and bedrock, potentially increasing contributions from locally derived mineral particles. How these local and remote dust sources vary seasonally, and how they are recorded in the mineralogical composition of snow-surface particles, remains poorly understood. This study aims to clarify the seasonal and spatial variability of mineral dust sources on alpine snow surfaces in the central Japanese mountains.

 We analyzed mineral particles deposited on snow surfaces in the Tateyama Mountains, central Japanese Alps. Surface snow samples collected during the melt season (May–July 2017) were compared with dust-layer samples from a snow pit excavated in April 2008, representing springtime deposition. Mineralogical analyses using X-ray diffraction and optical microscopy show that dust deposited in April and during the early melt season is dominated by quartz and feldspar, consistent with long-range transported mineral dust. As the melt season progressed, the relative abundances of Fe–Mg–bearing minerals, including chlorite, biotite, and amphibole, increased systematically. Spatial variations further reveal localized feldspar enrichment at specific sites, indicating increasing inputs from locally derived mineral particles sourced from surrounding bedrock.

 These results demonstrate a pronounced seasonal shift in mineral dust provenance on alpine snow surfaces, from dominantly long-range transported dust in spring to increasing local geological contributions during the melt season. Such changes in mineralogical composition may alter snow surface albedo and melt processes, highlighting the need to consider mineral dust composition, not only dust loading, when evaluating alpine snowmelt dynamics.

 

How to cite: Ataka, P., Sugiyama, R., Furukawa, N., and Takeuchi, N.: Seasonal variability of mineral dust composition on an alpine snowpack in the Tateyama Mountains, Japan , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3933, https://doi.org/10.5194/egusphere-egu26-3933, 2026.

Sand and dust storms (SDS) are among the most impactful atmospheric hazards, affecting air quality, climate, ecosystems, and socio-economic activities across continents. East Asia is one of the world’s major dust source regions, and recent observations indicate a renewed increase in SDS frequency and intensity since the mid-2010s, with several extreme events occurring in 2021, 2023, and 2025. This contribution presents recent advances in SDS early warning and forecasting developed at the WMO Asian Sand and Dust Storm Warning Advisory and Assessment System (SDS-WAS) Regional Center, hosted by the China Meteorological Administration.

 

We highlight progress in multi-source monitoring, multi-model forecasting, and artificial intelligence (AI) applications for SDS prediction. Satellite-based minute-scale dust identification has been achieved through multi-sensor data fusion, enabling near-real-time monitoring of dust severity and three-dimensional vertical structure by integrating satellite, lidar, radar, and ground-based observations. On the forecasting side, operational multi-model ensemble systems provide regional dust concentration, optical depth, emission, and deposition products. A machine-learning-based ensemble correction approach further improves surface dust concentration forecasts by optimally combining multiple models based on their historical performance.

 

In addition, an AI-driven global coupled aerosol–meteorology forecasting system has been developed, delivering 5-day, high-resolution forecasts of dust optical depth and surface concentrations. Case studies demonstrate that this system captures long-range dust transport from both Asian and Saharan sources, including events affecting Europe, with forecast skill exceeding that of several regional numerical models.

 

As a WMO SDS-WAS Asian Regional Center, we emphasize the importance of strengthening collaboration with the WMO SDS-WAS program and other regional nodes. Enhanced data sharing, harmonized observational datasets, and coordinated multi-model and AI-based forecasting efforts are essential to improve global SDS early warning capabilities. The experience gained in Asia offers valuable insights for Europe and other downwind regions, supporting transboundary aerosol monitoring, risk assessment, and mitigation strategies at the global scale.

How to cite: An, L.: Developments in Monitoring and Multi-Model Applications of Dust Weather in SDS-WAS ASIAN REGIONAL CENTER, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4602, https://doi.org/10.5194/egusphere-egu26-4602, 2026.

EGU26-4611 | ECS | PICO | AS3.5

Understanding Global Haboobs Using iDust 

Mei Chong and Xi Chen

Haboobs, dust storms triggered by convective cold pool outflows, contribute significantly to the global dust cycle and cause severe socioeconomic impacts through rapid visibility reduction and health hazards. However, haboob processes are inadequately represented in current reanalysis products (MERRA-2, EAC4) due to insufficient resolution to resolve mesoscale convection and hydrostatic dynamics that cannot properly describe the small-scale vertical motions. To date, haboobs have been studied primarily through individual cases and regional statistics, while systematic global-scale understanding remains lacking. This study investigates the global spatiotemporal patterns of haboobs and quantifies their contributions to dust emissions using the 12.5-km iDust model with analysis wind nudging. We perform multi-year global simulations, validate them against ground-based and satellite observations, and systematically identify and characterize haboob events worldwide. Our findings reveal global haboob patterns and their role in the dust cycle, advancing scientific understanding of convective dust processes.

How to cite: Chong, M. and Chen, X.: Understanding Global Haboobs Using iDust, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4611, https://doi.org/10.5194/egusphere-egu26-4611, 2026.

The characteristics and potential influence of dust events under the background of Northeast China Cold Vortex (NCCV) have rarely been investigated. Based on meteorological observational data and ERA5 reanalysis data from 2015 to 2023, we examined the spatiotemporal and environmental characteristics of dust events under NCCV and non-NCCV conditions and explored the potential impacts of the NCCV on dust events. The results indicate that dust days in Northeast China exhibited a trend of first decreasing and then increasing during the study period, and severe dust events mainly occurred in central Inner Mongolia, a key dust source region in China. Dust days associated with the NCCV accounted for 32.7% of the total dust days, and their station-frequency ratio reached 43.7%. Dust events were predominantly concentrated in the southwest quadrant of the NCCV periphery (60.1%), mostly within a range of 1.0–2.6 times the NCCV radius. This distribution pattern can be attributed to the strong baroclinity often related to the low-level shear lines and dry ambient conditions in this region. Moreover, strong downward momentum transfer and weakly stable stratification within the planetary boundary layer under NCCV conditions also facilitated the formation of dust events. This study reveals the important impacts of the NCCV on dust events, thereby providing a scientific basis for further understanding the formation mechanisms of such events.

How to cite: Li, X. and Xu, S.: Characteristics and impacts of dust events under the background of Northeast China Cold Vortex (NCCV), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5478, https://doi.org/10.5194/egusphere-egu26-5478, 2026.

EGU26-5689 | ECS | PICO | AS3.5

Re-evaluating Dust Emission Potential from Burned Surfaces on Vegetated Dunes in the Southwest Kalahari 

Rosemary Huck, Giles Wiggs, David Thomas, and Natasha Wallum

Sand dunes are not typically considered a major contributor to atmospheric dust loading due to coarse grain sizes and the infrequent observation of dust emission events. In vegetated dune systems, dust emission is less common as plant cover inhibits wind erosion. However, disturbances, such as fire, can rapidly remove protective vegetation cover which exposes resident fine sediments to wind erosion.

This study investigates dust emission potential following fire-induced de-vegetation in the driest region of the world’s largest sand sea, the southwest Kalahari. Adopting a hybrid approach, we combine remote sensing to characterise fire extent and timing and portable wind tunnel (PI-SWERL) experiments to quantify erosion potential.

A 24-year fire inventory reveals that burning is most frequent during or immediately after La Niña events, although anthropogenic land management significantly influences the spatial and temporal distribution of fires. The period for dust emission potential following fire is short, constrained by rapid vegetation recovery typically within 2 years. Grain size analyses indicate that dust-sized particles (<62.5 μm) are present in both burned and unburned dune surfaces; however, no significant depletion of fine particles from burned surfaces was observed, suggesting minimal loss through aeolian processes.

PI-SWERL experiments confirm that these fine particles can be entrained, yet higher threshold friction velocities are required for erosion at burned sites. The presence of biological soil crusts (biocrust) at all burned sites implies a stabilising influence on the erosion threshold. Where the surface had been disturbed, resulting in the removal of the typically present biocrust, our data suggest that dust emission fluxes are, on average, 8-13 times higher than those of unburned surfaces.

These findings indicate that currently there is little potential for dust emission in the post-fire de-vegetation period. This study provides new insights into the mechanisms controlling dust emissions in partially vegetated dune landscapes and highlights the importance of multiple, interacting, surface properties in governing aeolian processes.

How to cite: Huck, R., Wiggs, G., Thomas, D., and Wallum, N.: Re-evaluating Dust Emission Potential from Burned Surfaces on Vegetated Dunes in the Southwest Kalahari, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5689, https://doi.org/10.5194/egusphere-egu26-5689, 2026.

EGU26-6290 | PICO | AS3.5

Aridity record from the western Australia across the Early-Middle Pleistocene Transition 

Terezia Kunkelova, Anna Arrigoni, and Gerald Auer

Australian aridity is primarily governed by large-scale atmospheric circulation and by the influence of the Australian-Indonesian monsoon (AIM). Regional climate variability is further modulated by coupled ocean-atmosphere modes, including the El Niño-Southern Oscillation (ENSO), the Indian Ocean Dipole (IOD), and the Southern Annular Mode (SAM), whose interactions regulate moisture supply and hydroclimatic variability across the Australian continent. Western Australia has experienced pronounced hydroclimatic variability through time, characterized by arid glacial intervals and more humid interglacials, highlighting a strong regional sensitivity to insolation forcing, large-scale atmospheric circulation, and changes in Indo-Pacific climate modes. However, Australian hydroclimate responses during intervals of major climatic reorganization, such as the Early-Middle Pleistocene Transition (EMPT), remain poorly constrained. The EMPT (~1.2-0.6 Ma) marks a fundamental reorganization of the climate system, characterized by intensified glacial-interglacial cycles and a shift toward a ~100-kyr periodicity.

Here, we present a grain size record from IODP Site U1460 spanning the EMPT, reflecting changes in aridity within western Australia. Using a grain-size end-member unmixing model, we aim to distinguish relative changes in the proportions of fine-grained material and coarser-grained sediment as proxies for shifts between humid and arid intervals. Furthermore, we are developing a specialized method to remove biogenic silica from marine sediment, as the site contains a high concentration of sponge spicules. These spicules are particularly challenging to remove due to their chemical resilience. This method is critical to prevent interference with sedimentological measurements and to ensure the accuracy of our grain size end-member modelling and hydroclimatic interpretations. Our grain size record will not only provide a refined biogenic silica removal method but also offer new insights into the evolution of Australian arid environments and the mechanisms linking regional hydroclimate to global climate reorganization during the Pleistocene. These findings will serve as critical analogues for understanding hydroclimatic sensitivity under sustained anthropogenic forcing.

How to cite: Kunkelova, T., Arrigoni, A., and Auer, G.: Aridity record from the western Australia across the Early-Middle Pleistocene Transition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6290, https://doi.org/10.5194/egusphere-egu26-6290, 2026.

EGU26-7051 | ECS | PICO | AS3.5

Dust amplified Glacier Mass Loss in High Mountain Asia 

Xingli Mao

Dust aerosols impact High Mountain Asia (HMA) glacier mass balance through reducing albedo (direct effect) and affecting the accumulation of glacial materials by disturbing precipitation (indirect effect), but the mechanism remains unclear.  Using a regional climate model and coupling it to a glacier energy-mass balance model for the period 2016-2022, we demonstrate that dust amplifies glacier mass loss by 6%, primarily by reducing solid precipitation (46%) and albedo (41%). This dust-induced glacier retreat leads to significant declines in water storage, particularly in the Tarim Basin (-13%). As dust emissions are projected to rise, transboundary mitigation is urgently needed to preserve regional water security.

How to cite: Mao, X.: Dust amplified Glacier Mass Loss in High Mountain Asia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7051, https://doi.org/10.5194/egusphere-egu26-7051, 2026.

EGU26-7253 | PICO | AS3.5

Towards Understanding the Climate Response to the Historical Dust Increase in ICON-XPP 

Claus Sarnighausen, Natalia Sudarchikova, and Stephanie Fiedler

Mineral dust aerosol shapes the global climate, mainly through interactions with radiation and clouds, and especially on the regional level close to major emission sources. However, the Coupled Model Intercomparison Project, phase six (CMIP6) models with coupled dust emission parameterization schemes fail to reproduce the 55 ± 30% increase in atmospheric dust concentration since 1850 (Kok et al. 2023). In the present study, we construct the historically changing monthly 'Dust Plumes' (DuPlumes) climatology (Sudarchikova et al. in prep.) and investigate implications of changing dust aerosol for the global climate in ICON-XPP, Germany's designated model for CMIP7. DuPlumes consists of a parameterized analytical framework, originally designed for anthropogenic aerosols (Stevens et al. 2017).  To create the representation of natural desert-dust aerosols, this study utilizes reanalysis data of dust optical depth, measurement data of scattering properties, and a marine-core-based reconstruction of the historical trend. To constrain the spatial pattern of present-day optical depth by observation, we use data of four reanalysis products (CAMS, MERRA2, JAero, and NAAPS), monthly averaged for the decade around the year 2010 (2004–2015). Plume functions related to ten dust plumes globally are fitted to the data using a gradient descent algorithm. The fit achieves a spatial correlation of r=0.98 with the data, with maximum deviations in summer of 0.08, or 2% of maximum aerosol optical depth, which is smaller than the uncertainty measured across the reanalysis ensemble. Compared to the currently implemented static ICON-XPP dust climatology, the reanalysis ensemble and, subsequently, dust plumes suggest considerably higher optical depth (~0.1) in the Eastern Asian Taklamakan and Gobi Desert regions. The vertical profile is informed by the 2007–2019 climatology derived from Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) retrievals. We also include measurements of dust scattering properties from literature, including in-situ data and laboratory measurements. Ongoing work includes ICON-XPP experiments with dust optical properties represented by DuPlumes. These allow us to estimate the spatial pattern of effective radiative effects of the present-day natural dust relative to the pre-industrial levels.

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Kok, J.F., Storelvmo, T., Karydis, V.A., Adebiyi, A.A., Mahowald, N.M., Evan, A.T., He, C., Leung, D.M.: Mineral dust aerosol impacts on global climate and climate change. Nat Rev Earth Environ. 4, 71–86 (2023). https://doi.org/10.1038/s43017-022-00379-5

Stevens, B., Fiedler, S., Kinne, S., Peters, K., Rast, S., Müsse, J., Smith, S.J., Mauritsen, T.: MACv2-SP: A parameterization of anthropogenic aerosol optical properties and an associated Twomey effect for use in CMIP6. Geoscientific Model Development. 10, 433–452 (2017). https://doi.org/10.5194/gmd-10-433-2017

How to cite: Sarnighausen, C., Sudarchikova, N., and Fiedler, S.: Towards Understanding the Climate Response to the Historical Dust Increase in ICON-XPP, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7253, https://doi.org/10.5194/egusphere-egu26-7253, 2026.

EGU26-7557 | ECS | PICO | AS3.5

The impact of grid resolution on global dust emission potential 

Pascal Kunze, Bernd Heinold, and Ina Tegen

Due to its radiative effects, mineral dust constitutes a critical component in global aerosol climate models. However, the representation of dust emissions currently remains a substantial source of uncertainties in dust model simulations. Convective systems are major contributors to dust emission. Moist convection, however, is still a sub-grid scale process in most climate models, which has to be parameterized. Recent comparison studies between high-resolution, convection-resolving simulations and models with horizontal resolutions, that do not allow for considering moist convection explicitly, have revealed the model resolution as a key driver for the model uncertainties.  To further evaluate the impact of model resolution on dust emission, we conducted an analysis based on surface winds from two distinct modeling frameworks: (i) the coarse-resolution CMIP6 model ensemble, where convection is parameterized, and (ii) high-resolution ICON simulations from the DYAMOND (DYnamics of the Atmospheric general circulation Modeled On Non-hydrostatic Domains) project, which explicitly resolve moist convection. An indicator of dust emissions is the so-called dust emission potential, which is calculated offline for these different datasets and systematically evaluated for key global source regions. The analysis reveals pronounced regional and seasonal differences in the magnitude and characteristics of the modeled dust emission proxy. To investigate the origins of these uncertainties, we further compare the model outputs with high-resolution regridded data and analyze the diurnal cycle of dust emissions in selected source regions with a special focused investigation of the Central Asian dust sources. The results highlight the necessity of using high-resolution emission modeling in specific dust source regions to more accurately represent dust-generating processes and their climate impacts.

How to cite: Kunze, P., Heinold, B., and Tegen, I.: The impact of grid resolution on global dust emission potential, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7557, https://doi.org/10.5194/egusphere-egu26-7557, 2026.

EGU26-7724 | PICO | AS3.5

Real-time analysis of trace metals in air by microwave induced plasma time-of-flight mass spectrometry (mipTOF) 

Martin Tanner, Alexander Gundlach-Graham, Martin Rittner, Lorenz Gfeller, Jay Slowik, Andre Prevot, Ed Fortner, and John Jayne

Keywords: Mass Spectrometry, Real-Time, Trace Elements, Source Apportionment, Mobile

Determination of the elemental composition of airborne nanoparticles and micro-particles is essential to understand the source(s) of these particles and also to predict potential health effects.1 The most common approach to measure the metal content of air is to collect samples on filters and then analyze digests by ICP-MS; however, this strategy offers poor time resolution (e.g. days) and only provides bulk element composition information. To understand the spatiotemporal characteristics of the emission of metal-containing aerosols, which is key to assessing exposure, real-time analysis strategies are essential. Here, we report on the development of a microwave induced plasma time-of-flight mass spectrometer (mipTOF) used for the direct analysis of metal-containing airborne particles.

The mipTOF is a field-deployable trace-element mass spectrometer. It uses a nitrogen-sustained high-power plasma (MICAP, Radom Instruments)2, 3 to quantitatively vaporize and atomize aerosols with sizes from the ultrafine to PM10. Singly charged atomic ions are generated in the plasma with high efficiency (up to 99%), and then extracted into the mass spectrometer, where they are sorted according to mass-to-charge ratio and recorded. Ambient air is sampled into the plasma via a concentric pneumatic nebulizer set up as a Venturi pump5 at flowrates from 100-200 cm3/min. With the mipTOF, concentration LODs range from 10 ng/m3 (potassium) to 0.05 ng/m3 (lead) with a time resolution of 10 seconds. The high-sensitivity, high-speed metal-aerosol measurements possible with mipTOF enable new research into real-time spatiotemporal analysis of metals in air. We will report on the use of the mipTOF in mobile lab measurements in Switzerland and Massachusetts, USA. In these measurements, we identified several unique sources of airborne metals, including emissions from automotive brake wear, trains, metal-plating industries, cement manufacturers, and light aircraft. In addition to presenting data from these campaigns, we will discuss aspects of instrument design and operation, including power and size requirements, calibration strategies, and instrumental figures of merit.

References:

(1) Daellenbach, K. R. et al. Nature 2020, 587 (7834), 414-419.

(2) Jevtic, J.; Menon, A.; Pikelja, V. PCT/US14/24306, 2015.

(3) Schild, M. et al.  Analytical Chemistry 2018, 90 (22), 13443-13450.

(4) Nishiguchi, K.; Utani, K.; Fujimori, E. J. Anal. Atom. Spec. 2008, 23 (8), 1125-1129.

How to cite: Tanner, M., Gundlach-Graham, A., Rittner, M., Gfeller, L., Slowik, J., Prevot, A., Fortner, E., and Jayne, J.: Real-time analysis of trace metals in air by microwave induced plasma time-of-flight mass spectrometry (mipTOF), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7724, https://doi.org/10.5194/egusphere-egu26-7724, 2026.

Dust aerosols are a key component of the Earth's climate system. However, global climate models often depict mineral dust as a uniform aerosol. This simplification limits the physical realism of dust simulations, necessitating comparison with available observations to determine whether mineralogical variability is accurately represented when incorporated into a global climate-aerosol model.

In this study, we examine how well a mineralogical soil database translates into realistic mineral-resolved dust transport and deposition in the global climate model ICON coupled with the aerosol module HAM. This implementation is based on the mineralogical soil database of Journet et al. (2014), as modified by Goncalves-Ageitos et al. (2023), and it explicitly represents 12 individual minerals. Using multi-year global simulations, we evaluate the simulated mineralogical dust cycle with a focus on emission patterns, transport pathways, regional deposition, and the representation of seasonal and interannual variability. Model results are compared with available observations and datasets to assess the added value and limitations of mineral-resolved dust representation.

The evaluation demonstrates where mineralogical information helps to better constrain dust transport and deposition and identifies key uncertainties that remain. These results provide a basis for future work on mineral-specific dust deposition and its role in biogeochemical cycles.

How to cite: Hofmann, E., Wagner, R., and Schepanski, K.: How well does a mineralogical soil database translate into realistic mineral-resolved dust transport and deposition in a global climate model?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7789, https://doi.org/10.5194/egusphere-egu26-7789, 2026.

EGU26-9453 | PICO | AS3.5

Laboratory investigation of the radiative properties of mineral dust across the solar and terrestrial spectrum: key achievements and future directions 

Claudia Di Biagio, Pasquale Sellitto, Bénédicte Picquet-Varrault, Jean-François Doussin, and Paola Formenti

Coarse mineral dust aerosols originating from arid and semi-arid regions worldwide constitute one of the dominant tropospheric aerosol species by mass. Mineral dust both absorbs and scatters solar and terrestrial radiation, thereby influencing the radiance spectrum at the surface and at the top of the atmosphere, as well as the atmospheric heating rate. Dust is a key, yet still highly uncertain, contributor to both historical and contemporary climate change.

Modelling the interaction of dust with atmospheric radiation remains challenging because dust absorption and scattering properties, represented by the complex refractive index, depend on mineralogical composition – which varies with the emission source – and on particle size distribution, which evolves during transport. Climate models and remote-sensing retrievals therefore require accurate, regionally dependent information to improve dust representation and reduce uncertainties in radiative effect estimates.

Laboratory investigation has proven to be a powerful approach for unravelling the optical properties of mineral dust across the solar and terrestrial infrared spectrum. Original experiments based on realistic aerosols generated from natural soils have provided important new insights into the optical properties of global mineral dust in the solar and thermal infrared spectral ranges, as well as their variability with particle composition and during transport. These results have motivated the modelling and remote-sensing communities to revisit dust representation in models, leading to new evaluations of the dust direct radiative effect and its associated uncertainty, as well as to the development of innovative remote-sensing products. Current research is now extending the investigated spectral range toward the far infrared and to emerging source regions, for which knowledge of dust–radiation interactions remains very limited.

This presentation highlights key results and open scientific questions that have driven recent research on the radiative properties of mineral dust, and outlines perspectives for future studies.

How to cite: Di Biagio, C., Sellitto, P., Picquet-Varrault, B., Doussin, J.-F., and Formenti, P.: Laboratory investigation of the radiative properties of mineral dust across the solar and terrestrial spectrum: key achievements and future directions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9453, https://doi.org/10.5194/egusphere-egu26-9453, 2026.

EGU26-10457 | ECS | PICO | AS3.5

Tracing the provenance and evolution of Asian dust fluxes during the Holocene: A geochemical study of sediment archives from Adak Island, Alaska 

Rakesh Kumar Rout, Tolulope Joseph Ayodeji, Nicolas Waldmann, and Daniel Palchan

Asian dust plumes export micronutrients eastward to the Pacific Ocean and are substantial for regulating the marine biogeochemical cycles and productivity. Previous studies from the Gulf of Alaska (a high-nutrient and low-chlorophyll zone) revealed that the dominant nutrient supply during the last deglaciation was primarily sourced from iceberg meltwater instead of local Alaskan dust fluxes. However, attention to distal dust sources from Asia was limited, possibly due to resolution constraints. To address this, we consider here two chronologically well-constrained (by tephrochronology and radiocarbon dating) sedimentary archives from Adak Island (Andrew and Heart lakes), in the central Aleutian Islands, Alaska. These records preserve a high-resolution environmental and climatic history for the last ~10 ka and might also include a continuous record of Asian dust plume sources. Terrigenous materials in these sediments originate from either local weathered basalt units and volcanic ash or from distal Asian dust, comprising erosional products of the granitoid terrane. We studied the siliciclastic fraction of the sediments recovered from both lakes and employed elemental analyses along with radiogenic isotopes (Sr, Nd and Pb) to identify and quantify possible allochthonous dust sources. Our preliminary observations from major and trace elemental ratios and statistical analyses (PCA and factor loadings) suggest that, indeed, there are two dominant sources for terrigenous sediments. The enriched LREE and flat HREE pattern, together with a positive Eu anomaly, further support the mixed source (mafic to felsic) of the sediment supply to the lakes. Additionally, the Chemical Index of Alteration (CIA) and other elemental ratios in both lakes suggest a sharp decreasing trend ca. 4 ka followed by an increasing trend ca. 3.5 ka, which is asynchronous with the increased input of Asian dust and the neoglacial cooling event during this interval. The isotopic and other geochemical studies are in progress, which will further validate these findings.

How to cite: Rout, R. K., Ayodeji, T. J., Waldmann, N., and Palchan, D.: Tracing the provenance and evolution of Asian dust fluxes during the Holocene: A geochemical study of sediment archives from Adak Island, Alaska, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10457, https://doi.org/10.5194/egusphere-egu26-10457, 2026.

EGU26-10511 | PICO | AS3.5

Resolving regional controls on dust flux: High-resolution chronostratigraphy of Carpathian loess 

Zoran Perić, Slobodan Marković, Petar Krsmanović, Helena Alexanderson, and Milica Bosnić

Loess-palaeosol sequences (LPS) are vital among terrestrial archives for reconstructing Quaternary palaeoclimates and environmental change. Their extensive distribution across continental mid-latitudes and high sensitivity to atmospheric and surface processes make them indispensable records of past dust cycles, wind regimes, and regional ecosystem dynamics. However, the reliability of these reconstructions, particularly quantitative measures of dust flux variability, is intrinsically limited by the resolution and accuracy of the underlying geochronological framework. Our research directly addresses this chronometric challenge by applying refined luminescence dating techniques and Bayesian age-depth modelling to loess profiles across the Carpathian and Wallachian Basins. This methodological approach enables the construction of high-resolution, probabilistic chronologies that are essential for robust palaeoenvironmental interpretation. The central outcome of this work is a significantly improved, regional reconstruction of dust flux variability. Our integrated analysis demonstrates that dust mass accumulation rates (MARs) across the basins do not conform to a simplified model of peak deposition solely during glacial maxima (MIS 2). This pattern indicates that dust influx was not driven exclusively by global ice volume but was significantly intensified during specific phases of regional climatic amelioration. These findings compel a reinterpretation of regional atmospheric and sediment dynamics. The high dust fluxes during MIS 3 highlight the critical influence of regional controls, such as changes in palaeowind intensity and pathways, episodic sediment supply from major river systems, and the variable dust-trapping efficiency of sparsely vegetated, dynamic landscapes. This underscores the necessity of disentangling the effects of global climate drivers from those of local environmental and geomorphic settings when interpreting the LPS record. The broader objective of this synthesis is to establish a robust, integrated stratigraphic and chronological framework that enables detailed correlation and comparison of loess-derived palaeoenvironmental proxies across the Carpathian and Wallachian Basins. By doing so, we provide new insights into the timing, magnitude, and climatic forcing of past atmospheric dust activity, challenging purely glacially-driven models and contributing to a more nuanced understanding of Quaternary environmental dynamics in Central and Eastern Europe.

How to cite: Perić, Z., Marković, S., Krsmanović, P., Alexanderson, H., and Bosnić, M.: Resolving regional controls on dust flux: High-resolution chronostratigraphy of Carpathian loess, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10511, https://doi.org/10.5194/egusphere-egu26-10511, 2026.

EGU26-10600 | ECS | PICO | AS3.5

Improving dust emission in WRF-Chem GOCART scheme using a high-resolution erodibility dataset 

Leandro Segado-Moreno, Juan Pedro Montávez, Eloisa Raluy-López, Ginés Garnés-Morales, Alejandro Cordero, and Pedro Jiménez-Guerrero

Mineral dust is a major atmospheric aerosol, affecting climate, air quality, and human health through radiative and microphysical processes. The Iberian Peninsula is frequently impacted by dust intrusions from North Africa, leading to episodic exceedances of PM10 concentrations that challenge operational air quality forecasts. Accurate simulation of dust emission and transport remains difficult due to uncertainties in soil erodibility, land surface characteristics, and meteorological drivers.

In this study, we assess the impact of two newly developed high-resolution soil erodibility datasets on regional dust simulations using WRF-Chem with the GOCART scheme. The first dataset, EROD, improves dust source representation by integrating fine-resolution topography (GMTED2010), achieving 0.0625° (≈5 km) resolution globally and 1 km locally for the Iberian Peninsula. The second dataset, SOILHD, further refines dust source characterization by incorporating local-scale soil composition (sand, silt, clay fractions) and removing areas erroneously classified as bare soil, reaching 1 km resolution globally. These datasets aim to capture the spatial heterogeneity of dust sources, which is critical in semi-arid regions with sparse vegetation and variable soil properties.

We conduct WRF-Chem simulations for five periods between 2022 and 2025, representing a range of dust episodes with local and long-range transport. Model performance is evaluated against PM10 measurements from the SINQLAIR network across coastal and inland stations in the Region of Murcia. Results indicate that the high-resolution datasets substantially improve the spatial and temporal representation of dust emissions. Inland and low-anthropogenic-influence stations show better agreement with observed PM10 peaks in both magnitude and timing compared to simulations using standard coarse-resolution erodibility fields. At coastal and industrially influenced sites, improvements are more limited due to missing anthropogenic emissions and additional aerosol components, but statistical metrics such as correlation, Mean Bias Error (MBE), and Root Mean Square Error (RMSE) still indicate significant enhancement.

Overall, the results demonstrate that high-resolution, type–aware soil erodibility datasets significantly enhance the skill of dust simulations in WRF-Chem, reducing biases and capturing observed variability more accurately. These findings underscore the importance of detailed soil and topographic information for regional dust modeling and highlight the potential benefits of incorporating such datasets into operational dust forecasting systems.

How to cite: Segado-Moreno, L., Montávez, J. P., Raluy-López, E., Garnés-Morales, G., Cordero, A., and Jiménez-Guerrero, P.: Improving dust emission in WRF-Chem GOCART scheme using a high-resolution erodibility dataset, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10600, https://doi.org/10.5194/egusphere-egu26-10600, 2026.

EGU26-11564 | PICO | AS3.5

Dust-driven droplet freezing explains cloud-top phase in the northern extratropics. 

Diego Villanueva, Martin Stengel, Corinna Hoose, Kai Jeggle, Olimpia Bruno, Albert Ansmann, and Ulrike Lohmann

Clouds with temperatures between −39° and 0 °C can be capped by either a liquid or an ice layer, strongly influencing their radiative forcing and precipitation. The cloud-top ice-to-total frequency (ITF) quantifies the occurrence of clouds with ice tops relative to all clouds, yet the processes controlling ITF remain poorly understood. Using 35 years of satellite observations (Cloud_cci v3) and dust reanalysis (MERRA2), we show that in the Northern Hemisphere, at temperatures between −15° and −30 °C, ITF is strongly correlated with dust aerosol variability in both time and space. Moreover, we find that the sensitivities of ITF to temperature and dust occur in a ratio consistent with laboratory measurements of immersion droplet freezing, indicating that dust aerosols impose a logarithmic control on cloud-top phase.

How to cite: Villanueva, D., Stengel, M., Hoose, C., Jeggle, K., Bruno, O., Ansmann, A., and Lohmann, U.: Dust-driven droplet freezing explains cloud-top phase in the northern extratropics., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11564, https://doi.org/10.5194/egusphere-egu26-11564, 2026.

EGU26-12006 | PICO | AS3.5

 Dust source transfer from North Africa to the Amazon Basin: geochemical constraints on their long-term sources and composition  

Damien Guinoiseau, Christopher Pöhlker, Anna Kral, Jorge Saturno, Florian Ditas, Paulo Artaxo, Meinrat O. Andreae, and Stephen J.G. Galer

At a global scale, dust can serve as a vector for transferring elements from nutrient-rich soils to nutrient-depleted ecosystems, acting as a natural fertilizer [1]. The Amazonian rainforest, which is partly developed over nutrient-poor lateritic soils, illustrates this concept by receiving annually 8.5 Tg of dust from North African regions [2]. This phenomenon is well-documented and captured by both satellite-derived and in situ observations; however, the documentation of the long-term dust sources in North Africa and their associated chemical composition remains debated today [3,4]. This study presents two chronicles of dust collected at the Atmospheric Tall Tower Observatory (ATTO) during the dust-active season (February to April) in 2016 and 2017. Following a chemical extraction procedure already reported elsewhere [5], the chemical compositions and Sr-Nd-Pb isotope signatures of samples collected during low-dust conditions and dust outbreak events have been analyzed.

Following a statistical ACP and clustering analysis, the extracted water-soluble, acid-soluble, and residual fractions show that dust loading is the main driver of aerosol composition. Carbonated minerals do not survive efficiently in the atmospheric conditions encountered during transatlantic transport within the Saharan Air Layer and are readily solubilized. Most of the silicates and oxides are resistant to atmospheric chemical weathering, with the exception of poorly crystallized Al-Fe oxides. Finally, the geochemical signals of trace metals, potassium, and phosphorus can be complicated by anthropogenic particles or emitted bioaerosols, in addition to dust.

Predominant north African dust sources are identified by combining rare earth element patterns with Sr-Nd-Pb radiogenic isotopes, both of which are clearly diagnostic. A Bayesian mixing model (MixSIAR) is also used to quantify the long-term proportion of each source, while satellite products (CALIPSO, MERRA-2) and back trajectory analyses (HYSPLIT) are used to confirm our observations. Western African soils characterized by alluvial deposits in wadis developed over Phanerozoic terrains are the dominant dust sources (55-90%), while soils associated with Precambrian cratonic areas can act sporadically during significant dust events. As already postulated using a satellite-derived model [3], the Bodélé Depression’s impact on dust reaching the Amazon Basin is negligible, despite its status as the dustiest place on Earth. These results are consistent with conclusions drawn for the Northern Hemisphere, particularly for the Caribbean [5], although dust transport and atmospheric conditions over North Africa differ seasonally (between boreal winter and boreal summer). Finally, the chemical composition of the dust measured for all dust events reaching ATTO in 2016 and 2017 is remarkably uniform and consistent with 2024 and 2025 collected samples from French Guiana and ATTO (Collignon et al., in prep.), allowing for a preliminary estimate of a long-term “averaged North African dust” composition reaching the Amazon Basin.

[1] Reicholf (1986), SNFE, 21, 251-255.

[2] Kok et al. (2021), ACP, 21, 8169-8193.

[3] Yu et al. (2020), GRL, e2020GL088020.

[4] Barkley et al. (2022), GRL, e2021GL097344.

[5] Kumar et al. (2018), EPSL, 487, 94-105.

How to cite: Guinoiseau, D., Pöhlker, C., Kral, A., Saturno, J., Ditas, F., Artaxo, P., Andreae, M. O., and Galer, S. J. G.:  Dust source transfer from North Africa to the Amazon Basin: geochemical constraints on their long-term sources and composition , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12006, https://doi.org/10.5194/egusphere-egu26-12006, 2026.

EGU26-12288 | ECS | PICO | AS3.5

The chemical and mineralogical composition of southern African dust aerosols 

Clarissa Baldo, Sophie Nowak, Servanne Chevaillier, Gael Noyalet, Silvia Becagli, Akinori Ito, Sandra Lafon, Claudia Di Biagio, Karine Desboeufs, Remi Stanus, Nadine Mattielli, Heleen C. Vos, Gregory S. Okin, James S. King, Amelie Chaput, Brigitte Language, Stuart Piketh, and Paola Formenti

Southern Africa (SAf) is a key region for dust emissions, characterised by a wide variety of natural and anthropogenic sources, but also a critical knowledge gap in the mineral dust budget of the Southern Hemisphere. Projected climate warming is expected to lead to an increase in mineral dust emissions, which are increasingly linked to human activity. Although the transport and deposition pathways of SAf dust suggest that it can directly affect the regional climate and nearby marine ecosystems through dust-aerosol interaction and indirectly through aerosol-cloud/ice interaction and nutrient deposition, the extent of this impact is highly uncertain due to significant uncertainties in atmospheric loads and climate-relevant properties.

This study provides the first comprehensive characterisation of the chemical and mineralogical composition of SAf dust aerosols. Aerosol samples were laboratory-generated using soils collected from key dust sources in southern Africa, including the Namib gravel plain, coastal ephemeral riverbeds, the Etosha salt pan, the Kalahari Desert, and anthropogenic sources such as agricultural soils from the Free State, savannah soils from the Kruger National Park, and a copper mine in Namibia.

A geographical distribution of the chemical and mineralogical properties of SAf dust was identified based on the elemental ratios Si/Al, (Ca + Mg)/Al, and K/Al. This is influenced by both the regional geology and rainfall distribution, which shows an increase in the Si/Al ratio and a decrease in the (Ca + Mg)/Al and K/Al ratios, in areas with higher rainfall inland compared to the arid coast, while the salt pans exhibit unique features with significantly higher (Ca+Mg)/Al and Si/Al ratios.

The SAf dust appears to be more enriched in Ca, Mg, and K than other dust sources in the Southern Hemisphere and northern African dust. Although Fe, a key micronutrient, occurs at similar levels in dust from both hemispheres, SAf dust contains more P, highlighting its potential significance in biogeochemical cycling. Despite limited mineralogical observations in the Southern Hemisphere, our results indicate that SAf dust contains more feldspar minerals than northern African dust, and may strongly influence the load of ice-nucleating particles over the Southern Ocean and, in turn, the regional radiative budget.

How to cite: Baldo, C., Nowak, S., Chevaillier, S., Noyalet, G., Becagli, S., Ito, A., Lafon, S., Di Biagio, C., Desboeufs, K., Stanus, R., Mattielli, N., Vos, H. C., Okin, G. S., King, J. S., Chaput, A., Language, B., Piketh, S., and Formenti, P.: The chemical and mineralogical composition of southern African dust aerosols, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12288, https://doi.org/10.5194/egusphere-egu26-12288, 2026.

In the temperature range between 0 °C and −39 °C, clouds may exist in the liquid phase, the ice phase, or as a mixture of both. Cloud glaciation, defined as the transition from liquid to ice, can be driven by multiple processes. On the one hand, enhanced glaciation may result from secondary ice production. On the other hand, atmospheric aerosols can act as ice-nucleating particles (INPs) and initiate ice crystal formation. Previous studies have highlighted the role of mineral dust as the dominant INP source for cloud glaciation at temperatures below −15 °C.

Although recent findings indicate a correlation between aerosol concentration and cloud glaciation, quantifying aerosol–cloud interactions remains challenging. To better characterize and disentangle the natural spatial and temporal variability of relevant observables governing this relationship, this study combines data from multiple satellite instruments (MSG SEVIRI, MODIS, and IASI). In addition, these observations are compared to ICON model outputs and CAMS reanalysis data. The objective is to provide an assessment of the sensitivity of cloud phase to dust aerosol concentration for given temperatures and synoptic conditions across different datasets.

We primarily investigate the influence of the dust aerosol optical depth (DAOD) in the region between the equator and the subtropical dust belt (0–30° N/S). Our findings highlight the relationship between DAOD and cloud glaciation, characterized by a particularly strong increase in glaciation at high DAOD values. The analysis further includes stratification by large-scale synoptic conditions and cloud type, allowing us to narrow down potential differences between convective and stratiform clouds.

Finally, we examine how the integration of vertical profiles from EarthCARE may facilitate the detection of not only horizontally but also vertically collocated cloud and aerosol layers, thereby improving statistical estimates of aerosol–cloud interactions.

How to cite: Brüning, S., Stengel, M., and Robbins, D.: Investigating dust aerosol effects on mixed-phase cloud glaciation based on an intercomparison of satellite observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12744, https://doi.org/10.5194/egusphere-egu26-12744, 2026.

EGU26-13178 | ECS | PICO | AS3.5

Impact of iron-containing dust on atmospheric oxidation processes 

Simon Rosanka, Klaus Klingmüller, Rolf Sander, Andrea Pozzer, Jos Lelieveld, and Domenico Taraborrelli

In the atmosphere, organic and inorganic compounds can partition into clouds, fog, raindrops, and aqueous aerosols, where they undergo rapid chemical oxidation, yielding secondary aerosols. This process is governed by the availability of radicals such as hydroxyl (OH) and nitrate (NO3) radicals in the liquid phase. The presence of dissolved iron can boost the OH reactivity via Fenton reactions. Dust is a major source of iron in the atmosphere, occurring primarily in the crystalline lattices of aluminosilicates or as iron oxides. Following its emission, iron tends to be mostly insoluble but can be converted into soluble forms when inorganic acids decrease the pH, and organic ligands create iron complexes during atmospheric transport. In this study, we address the importance of iron in global atmospheric oxidation processes by mechanistically modelling the related chemical processes in the gas and liquid phases within clouds, fog, rain droplets, and, for the first time, aqueous aerosols. We employ the atmospheric chemistry MESSy model infrastructure, coupled to the global general circulation model ECHAM5 (EMAC). We represent three mechanisms of iron dissolution into aerosol water, driven by aerosol acidity, irradiation, and the presence of oxalate in the solution, which acts as an organic ligand. In the atmosphere, oxalate is the dominant dicarboxylic acid, mainly formed via aqueous-phase oxidation of glyoxal and other organic compounds. Our new approach is to explicitly account for oxalate-related aqueous-phase chemistry. Through a series of sensitivity simulations, with and without soluble iron, we address the global impact of iron on aqueous-phase oxidation capacity. We find that iron uptake into aerosol water enhances OH reactivity, particularly in cloud droplets, thereby increasing the aqueous oxidation of isoprene oxidation products and influencing secondary organic aerosol formation.

How to cite: Rosanka, S., Klingmüller, K., Sander, R., Pozzer, A., Lelieveld, J., and Taraborrelli, D.: Impact of iron-containing dust on atmospheric oxidation processes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13178, https://doi.org/10.5194/egusphere-egu26-13178, 2026.

EGU26-13316 | PICO | AS3.5

Transported African Dust in the Lower Marine Atmospheric Boundary Layer is Internally Mixed with Sea Salt Contributing to Increased Hygroscopicity and a Lower Lidar Depolarization Ratio 

Cassandra Gaston, Sujan Shrestha, Robert Holz, Willem Marais, Zachary Buckholtz, Ilya Razenkov, Edwin Eloranta, Jeffrey Reid, Hope Elliott, Nurun Nahar Lata, Zezhen Cheng, Swarup China, Edmund Blades, Albert Ortiz, Rebecca Chewitt-Lucas, Alyson Allen, Devon Blades, Ria Agrawal, Elizabeth Reid, and Jesus Ruiz-Plancarte and the Ragged Point MAGPIE Team

Saharan dust is frequently transported across the Atlantic, yet the chemical, physical, and morphological transformations dust undergoes within the marine atmospheric boundary layer (MABL) remain poorly understood. These transformations are critical for understanding dust’s radiative and geochemical impacts, it’s representation in atmospheric models, and detection via remote sensing. Here, we present coordinated observations from the Office of Naval Research’s Moisture and Aerosol Gradients/Physics of Inversion Evolution (MAGPIE) August 2023 campaign at Ragged Point, Barbados. These include vertically resolved single-particle analyses, mass concentrations of dust and sea spray, and High Spectral Resolution Lidar (HSRL) retrievals. Single-particle data show that dust within the Saharan Air Layer (SAL) remains externally mixed, with a corresponding high HSRL-derived linear depolarization ratio (LDR) at 532 nm of ~0.3. However, at lower altitudes, dust becomes internally mixed with sea spray, and under the high humidity (>80%) of the MABL undergoes hygroscopic growth, yielding more spherical particles, suppressing the LDR to <0.1; even in the presence of  high dust loadings (e.g., ~120 µg/m3). This low depolarization in the MABL is likely due to a combination of the differences between the single scattering properties of dust and spherical particles, and the potential modification of the dust optical properties from an increased hygroscopicity of dust caused by the mixing with sea salt in the humid MABL. These results highlight the importance of the aerosol particle mixing state when interpreting LDR-derived dust retrievals and estimating surface dust concentrations in satellite products and atmospheric models.

How to cite: Gaston, C., Shrestha, S., Holz, R., Marais, W., Buckholtz, Z., Razenkov, I., Eloranta, E., Reid, J., Elliott, H., Lata, N. N., Cheng, Z., China, S., Blades, E., Ortiz, A., Chewitt-Lucas, R., Allen, A., Blades, D., Agrawal, R., Reid, E., and Ruiz-Plancarte, J. and the Ragged Point MAGPIE Team: Transported African Dust in the Lower Marine Atmospheric Boundary Layer is Internally Mixed with Sea Salt Contributing to Increased Hygroscopicity and a Lower Lidar Depolarization Ratio, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13316, https://doi.org/10.5194/egusphere-egu26-13316, 2026.

EGU26-13474 | ECS | PICO | AS3.5

Unraveling the geochemical signals from major episodes of Saharan dust at two different locations in the Amazon basin. 

Lea Collignon, Damien Guinoiseau, Kathy Panechou, Cassandra J. Gaston, Sebastian Brill, Stephen J.G. Galer, Suresh Karunanithi, Christopher Pohlker, and Cecile Quantin

Desert dust is the most abundant aerosol by mass in Earth’s atmosphere (global dust loading of 22-29 Tg; [1]). One key region of interest is the Amazon Basin, which acts as a major sink for mineral dust transported from North Africa (deposition flux of ∼10 Tg.yr-1; [1]), impacting the nutrient supply to this rainforest ecosystem [2]. Currently, Western African sources are expected to be the predominant dust source based on previous geochemical studies [3] and atmospheric modeling [4], while the contribution of the Bodélé region is highly debated [4]. However, further constraints are still needed to elucidate the nutrient bioavailability associated with dust and other aerosol types, as well as how chemical transformations may affect the dust geochemical signal during transport and continentalization.

This study focuses on simultaneous high-resolution records of North African dust episodes reaching two different South American locations from January to March 2025. The first location is a coastal observatory in French Guiana (ATMO), while the second is located in the central Amazon forest, in Brazil (ATTO). Although these observatories are separated by more than 1,000 km, they are both influenced by similar transatlantic air mass trajectories, enabling an assessment of the impact of air mass continentalization on the chemical and physical characteristics of the aerosol particles. Aerosol samples have been chemically characterized using a recently developed selective extraction protocol [3], which segregates particles into water-soluble, acid-soluble, and residual material, including the silicate fraction of dust [5].

A 65 % dust loading reduction is observed between ATMO and ATTO sites, accompanied by a decrease in the soluble fraction from 20–50 %, dominated by sea salt at ATMO, to less than 10 % at ATTO. Other constituents originate from the dissolution of carbonates (Ca, Mg) due to atmospheric processes, from the leaching of soot particles or the emission of bioaerosols (K, P), and from the partial dissolution of poorly crystallized oxides (Al, Fe).  

The silicate fraction, which dominates the aerosol mass (50-98%), reveals a remarkable stability in the elemental composition of dust, irrespective of the observatory location, the position within the dust event (onset, peak, or decay), or the meteorological conditions. This compositional consistency exhibits a highly coherent signal when compared with previous dust episodes observed in 2016, 2017, and 2024 [3]. Furthermore, isotopic signatures of Sr, Nd, and Pb, known as efficient proxies for dust sources, are in strong agreement with those measured during these earlier episodes, confirming the dominant role of the West African dust source and the negligible contribution of the Bodélé Depression. Overall, these findings underscore the robust stability of the geochemical signal carried by dust, thereby enhancing our understanding of the average dust composition that reaches the Amazon Basin. In contrast, the focus on more labile components is strategic since these elements are preferentially redistributed into the water- and acid-soluble fractions.

 

[1] Kok et al. (2021), https://doi.org/10.5194/acp-21-8169-2021

[2] Swap et al. (1992), https://doi.org/10.1034/j.1600-0889.1992.t01-1-00005.x

[3] Collignon et al., submitted.

[4] Yu et al. (2020), https://doi.org/10.1029/2020GL088020

[5] Kumar et al. (2018), https://doi.org/10.1016/j.epsl.2018.01.025

 

How to cite: Collignon, L., Guinoiseau, D., Panechou, K., Gaston, C. J., Brill, S., Galer, S. J. G., Karunanithi, S., Pohlker, C., and Quantin, C.: Unraveling the geochemical signals from major episodes of Saharan dust at two different locations in the Amazon basin., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13474, https://doi.org/10.5194/egusphere-egu26-13474, 2026.

EGU26-14556 | ECS | PICO | AS3.5

Loess deposits record stable Mid-Pleistocene hydroclimate during phases of human occupation of Central Asia 

Ramona Schneider, Ekaterina Kulakova, Daniel Topal, Bjarne Almqvist, Jan-Pieter Buylaert, Farhad Khormali, Mads Faurschou Knudsen, Rezhep Kurbanov, Aske Lohse Sørensen, Gábor Újvári, David Keith Wright, Qiuzhen Yin, and Thomas Stevens

Palaeolithic tools preserved in the loess-palaeosol sections of southern Tajikistan as early as ~800 ka evidence the episodic presence of ancient hominins across major Quaternary climate shifts, such as the Mid-Pleistocene and Mid-Brunhes Transitions (MBT). The richest assemblage of lithic tools found in the region, the Karatau Culture, is found mainly in palaeosols associated with Marine Isotope Stages (MIS) 15, 13, and 11, with intervening glacial periods as well as previous and subsequent interglacial periods characterised by a near absence of tools, except for MIS 14 which contains a smaller number of artefacts. Curiously, the disappearance of the Karatau culture coincides with an abrupt increase in magnetic susceptibility in the palaeosol units. Currently, the cause of the alternating phases of occupation and their possible connection to wider-scale climate remain unclear.

The Khovaling Loess Plateau loess-palaeosol sequences provide an opportunity to understand the climatic and environmental context of the appearance and disappearance of early hominins. Since the Khovaling Loess Plateau is located in a transitional zone between climate systems (Mid-Latitude Westerlies, Siberian High and Indian Monsoon) regional climate may be sensitive to global climate reorganisations within the Quaternary. Based on the observed abrupt increase in magnetic susceptibility following MIS 11, it has been hypothesized that monsoon incursions may have occurred during some interglacials, and that these incursions may have ceased after MIS 11, coinciding with the disappearance of the Karatau culture. However, evidence for potential monsoon incursions is highly debated, and the cause for the change in the magnetic susceptibility record remains unclear. In this study, we apply a novel multi-frequency magnetic susceptibility approach, complemented by elemental composition data from XRF and XRD, and by paleoclimate simulations, to investigate possible variations of the hydroclimate in Central Asia. The simulations, performed with the fully-coupled HadCM3 global climate model, allow us to assess the relative and combined effects of orbital, greenhouse gas and ice sheet forcings on the hydroclimate variability including possible moisture transport pathway changes in Central Asia around MIS 13 and 11.

Based on the combined evidence, we argue that the abrupt increase in bulk magnetic susceptibility after MIS 11, observed across different sites in southern Tajikistan, is best explained by a sediment provenance change. It appears to be unrelated to any change in rainfall seasonality, and to a lesser degree, intensity. We demonstrate that relative frequency dependence of magnetic susceptibility (χFD %) is the most suitable proxy for calculating quantitative palaeoprecipitation estimates in this region. Our magnetic susceptibility results, calibrated against a modern-analogue based transfer function, indicate that the demise of the Karatau culture coincides with an approximate +25% increase in regional annual mean precipitation. Combined with the other proxy data, this result indicates a relatively stable regional climate across periods of hominin occupation and the MBT.

How to cite: Schneider, R., Kulakova, E., Topal, D., Almqvist, B., Buylaert, J.-P., Khormali, F., Faurschou Knudsen, M., Kurbanov, R., Sørensen, A. L., Újvári, G., Wright, D. K., Yin, Q., and Stevens, T.: Loess deposits record stable Mid-Pleistocene hydroclimate during phases of human occupation of Central Asia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14556, https://doi.org/10.5194/egusphere-egu26-14556, 2026.

EGU26-14701 | PICO | AS3.5

Trace metal-containing aerosols in the atmosphere of the Indian Ocean 

Johannes Passig, Aleksandrs Kalamašņikovs, Haseeb Hakkim, Robert Irsig, Sven Ehlert, Andreas Walte, Eric Achterberg, and Ralf Zimmermann

Atmospheric deposition of aerosols constitutes a major source of iron and other micronutrients to remote ocean regions, where nutrient limitation constrains primary productivity and carbon sequestration. However, large uncertainties persist due to sparse observational data and the lack of sensitive techniques capable of resolving metal solubility at low aerosol loadings. Here we present first results from a shipborne campaign conducted aboard R/V Sonne across the Indian Ocean in late 2024 within the framework of the GEOTRACES program.

Aerosol particles were characterized using a novel single-particle mass spectrometer (SPMS) employing resonant laser ionization, enabling the analysis of the chemical composition of several hundred thousand individual particles. While sea spray aerosols dominated the overall particle population, thousands of iron-containing particles were detected, primarily associated with long-range transported mineral dust. Notably, a subset of sea spray aerosol particles exhibited detectable iron signals, suggesting in-cloud mixing or surface re-emission processes as potential sources.

For mineral dust particles, nitrate represented the dominant secondary component even in air masses without continental influence for more than ten days. Elevated iron contents within dust particles frequently coincided with the presence of dicarboxylic acids, whereas Mg/Ca-rich particles were preferentially associated with sulfate, indicating distinct atmospheric processing pathways, transport histories, and likely differences in iron solubility. By resolving such internal mixtures at the single-particle level, the SPMS provides a powerful approach for source attribution and for assessing the potential bioavailability of aerosol-derived metals. These observations reveal an unexpectedly high abundance and chemical diversity of iron-containing aerosols over the Indian Ocean, underscoring their importance for ocean biogeochemistry and nutrient cycling in this understudied region.

How to cite: Passig, J., Kalamašņikovs, A., Hakkim, H., Irsig, R., Ehlert, S., Walte, A., Achterberg, E., and Zimmermann, R.: Trace metal-containing aerosols in the atmosphere of the Indian Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14701, https://doi.org/10.5194/egusphere-egu26-14701, 2026.

EGU26-16641 | ECS | PICO | AS3.5

Size-resolved mineralogy and grain size-shape analysis of airborne and deposited mineral dust in northern China 

Katja Bohm, Hui Tang, Bin Wang, Sergio Andò, Anu Kaakinen, Thomas Stevens, Johanna Salminen, Ove Haugvaldstad, Eduardo Garzanti, and Jianrong Bi

The chemical and physical properties of atmospheric mineral dust play a key role in determining its climatic and environmental effects. These properties also vary globally, highlighting the importance of observational studies and regional investigations in enhancing global models. One of the major global dusty regions is Central-East Asia, where severe dust events occur frequently. It also hosts the largest terrestrial mineral dust record on Earth, the Chinese Loess Plateau (CLP), where dust has been deposited over the past 2.6 million years and beyond. The CLP region thus offers a globally unique archive to investigate the role of dust in both past and present climate states.

In this ongoing project, dust was collected in 2019–2021 by passive and active dust samplers from a total of six locations across the CLP region. Active collectors were placed at the Lanzhou University Semi-Arid Climate and Environment Observatory (SACOL; Gansu) and in the Shapotou District of Zhongwei (Ningxia) in the southeastern margin of the Tengger Desert. Passive samplers were placed at SACOL, Lingtai (Gansu), Yinchuan (Ningxia), Luochuan (Shaanxi), and Fugu (Shaanxi).

Grain size distributions and grain shape parameters (e.g., circularity, convexity, elongation) were measured simultaneously by Dynamic Image Analysis (DIA), while magnetic susceptibility measurements were also applied to the samples. The mineralogy of different size fractions was analysed using a single grain approach by Raman spectroscopy in the 2–10, 10–20, 20–63, and >63 µm grain size windows. Future investigations will include X-ray diffraction mineralogical analysis of the <2 µm fraction.

Temporal variations with up to daily resolution of the above-mentioned dust properties were studied from the Shapotou site, and initial magnetic susceptibility analyses suggest a change in the iron oxide composition and/or grain size during a severe dust storm event in March 2021. Future analyses will combine dust source contribution modelling and sedimentological dust provenance studies to better understand the dust cycle in Central-East Asia and its driving forces. We will also use the information on the modern dust properties and provenance to enhance understanding of the past Central-East Asian dust cycle during varying global climate states in Earth’s history and during the formation of the CLP. These include periods of warmer global climates that can be considered analogous to future conditions on our planet.

How to cite: Bohm, K., Tang, H., Wang, B., Andò, S., Kaakinen, A., Stevens, T., Salminen, J., Haugvaldstad, O., Garzanti, E., and Bi, J.: Size-resolved mineralogy and grain size-shape analysis of airborne and deposited mineral dust in northern China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16641, https://doi.org/10.5194/egusphere-egu26-16641, 2026.

EGU26-17511 | ECS | PICO | AS3.5

Late Pleistocene dust imprint in coastal dune archives spanning from the Canary to the Tyrrhenian Basin - Preliminary results 

Carsten Marburg, Andreas Gärtner, Heino Schäfer, Anja Maria Schleicher, Dominik Faust, and Christopher-Bastian Roettig

Saharan dust input is a well-known phenomenon worldwide but especially concerning landscapes around the Mediterranean Sea and on the Canary Islands since the largest dust source areas on earth are located in the Northern African continent. This dust transport is not just a recent process but has also been going on for the last glacial period with changing intensities. The availability of dust depends mainly on the vegetation cover in the source areas as well as changing wind strengths/pathways and is therefore a function of changing climate. Its effects have been imprinted in several geoarchives and are also well known from aeolianites. These coastal dune archives typically form in dependence of changes in sea level and are comprised of pale coloured carbonate sands, intercalated by reddish silty layers. The reddish silty layers are heavily influenced by dust imprint from the Northern African continent. The presented research project hence focuses on conducting detailed analyses on those layers to reconstruct the local and supraregional environmental conditions during the last glacial.
Our sites on the eastern Canary Islands (Lanzarote, Fuerteventura), SE-Spain, Balearic Islands (Formentera, Eivissa) and Sardinia offer best conditions to
(i) Analyse site-specific characteristics of the dust enriched layers and the stored information about the local environmental conditions,
(ii) Look for differences or systematical similarities in terms of quantities and admixture of dust material when comparing the different silty layers within a single site/profile,
(iii) Identify distinct source areas of dust as well as dominating dust pathways and
(iv) Correlate the different sites from the Canary to the Tyrrhenian basin and deduce supraregional patterns.
So far we conducted extensive fieldwork at all sites and realised a variety of laboratory analyses on samples from the Balearic Islands, for example grain-size specific heavy mineral, XRF-, XRD- and grain-size analysis. With our first results we identified dust enriched layers and utilised analysis of heavy mineral compositions as an additional method to trace possible dust source areas. With this we hope to contribute to the understanding of the large-scale development in the Western Mediterranean region and the Canary Islands during the last glacial.

How to cite: Marburg, C., Gärtner, A., Schäfer, H., Schleicher, A. M., Faust, D., and Roettig, C.-B.: Late Pleistocene dust imprint in coastal dune archives spanning from the Canary to the Tyrrhenian Basin - Preliminary results, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17511, https://doi.org/10.5194/egusphere-egu26-17511, 2026.

EGU26-18628 | ECS | PICO | AS3.5

How well do climate models represent dust events over the Mediterranean, North Africa, and the Middle East? 

Faidon Mavroudis, Antonis Gkikas, Donifan Barahona, Marı́a Gonçalves Ageitos, Danny Leung, Carlos Pérez Garcı́a-Pando, Ove Westermoen Haugvaldstad, and Georgia Sotiropoulou

Dust aerosols constitute a key component of the Earth–atmosphere system, affecting the radiation budget, the microphysical and optical properties of clouds, air quality, terrestrial and aquatic processes, and human health. Dust-related impacts are critically governed by the atmospheric load of mineral particles and are amplified when the dust burden substantially exceeds background levels. Such conditions, commonly referred to as episodes or events, are exceptional and characterized by pronounced spatiotemporal heterogeneity.

In this study, we present an intercomparison of three state-of-the-art climate models (EC-Earth3, CESM2, and NorESM2) and the GiOcean Reanalysis in representing dust events over the Mediterranean, North Africa, and the Middle East during the period 2003–2018. A percentile-based threshold methodology is applied to  daily dust optical depth (DOD) and aerosol optical depth (AOD) values, at both the grid-cell and regional scales, to identify three intensity-based episode categories: weak, moderate and extreme.  In addition, the satellite-based MIDAS dataset, which provides columnar DOD at 550 nm, is used as a reference for model evaluation.

The primary objective of this study is to assess inter-model differences in the representation of dust episode frequency of occurrence and intensity across multiple spatiotemporal scales, considering both free-running and nudged model configurations. Our working framework enables a comprehensive analysis by: (i) evaluating the ability of state-of-the-art climate models to represent different dust episode regimes, and (ii) investigating how threshold definitions influence the resulting spatiotemporal patterns of dust episodes. Finally, the outcomes of this study are expected to substantially enhance understanding of the strengths and limitations of climate models in depicting dust episode characteristics, thereby supporting improved projections under different climate scenarios throughout the 21st century.

How to cite: Mavroudis, F., Gkikas, A., Barahona, D., Gonçalves Ageitos, M., Leung, D., Garcı́a-Pando, C. P., Haugvaldstad, O. W., and Sotiropoulou, G.: How well do climate models represent dust events over the Mediterranean, North Africa, and the Middle East?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18628, https://doi.org/10.5194/egusphere-egu26-18628, 2026.

EGU26-18712 | ECS | PICO | AS3.5

A sink-to-source reverse approach to identify dust source regions within the Sahara based on PM₁₀ levels measured on the West African coast 

Marie Madeleine Atome Bassene, Aloys Bory, Moctar Camara, Yevgeny Derimian, Jean-Eudes Petit, Jean-Louis Rajot, Beatrice Marticorena, Laurine Verfaille, Dioncounda Yock, Fode Sambou, Thierno Mamadou Ndiaye, Aboubacry Diallo, and Viviane Roumazeilles

West Africa is a key region for the transport and deposition of Saharan mineral dust, with major impacts on air quality, climate, and ecosystems. Dust sources are numerous within the Sahara and their spatial extent remains poorly constrained, as do their granulometric, mineralogical, and chemical characteristics, which however control their impacts. Moreover, emission maps available in the literature do not allow the relative contribution of different source regions to a given impacted area to be assessed.

This study proposes a sink-to-source reverse approach aimed at improving the characterization of dust emission areas affecting the coastal West Africa. It is based on a three-year time series of PM₁₀ concentrations measured in Casamance, southern Senegal, a region under the influence of easterly winds (Harmattan) responsible for the transport of Saharan dust in the lower troposphere during the dry season. The measurements were conducted at a rural site (Pointe Saint Georges), minimally influenced by local and anthropogenic emissions.

PM₁₀ concentrations were coupled with air mass back-trajectories calculated using the HYSPLIT model and analyzed with the ZeFir software in order to identify potential source regions. Preliminary results suggest that, during high PM₁₀ concentration events observed along the West African coast, dust derived from two dominant sectors : one to the north-east including areas in Mauritania and across the Algerian-Mali border, and one to the east across the Sahelian region, confirming earlier findings (Le Quilleuc et al., 2021, JGR, doi.org/10.1029/2021JD035030). These results will be discussed in the light of emission areas provided by the satellite-based IDDI (Infrared Difference Dust Index) product as well as data on dust sources from the literature.

The results that will be presented highlight the potential of this sink-to-source approach for identifying mineral dust source areas based on airborne concentrations. This methodology, relying on low-cost sensors, is reproducible and applicable to any site located downwind of desert regions.

Keywords : PM₁₀, Saharan dust, Casamance, Senegal, air mass back-trajectories, HYSPLIT, ZeFir software, IDDI, sources

How to cite: Bassene, M. M. A., Bory, A., Camara, M., Derimian, Y., Petit, J.-E., Rajot, J.-L., Marticorena, B., Verfaille, L., Yock, D., Sambou, F., Ndiaye, T. M., Diallo, A., and Roumazeilles, V.: A sink-to-source reverse approach to identify dust source regions within the Sahara based on PM₁₀ levels measured on the West African coast, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18712, https://doi.org/10.5194/egusphere-egu26-18712, 2026.

EGU26-19014 | ECS | PICO | AS3.5

Fewer Dust Storms, Greater Dust Concentration in the Air 

Alaa Mhawish, Udaya Bhaskar Gunturu, Saud Alamoudi, Sultan Alduaji, and Jumaan Alqahtani

Recent observations over the Arabian Peninsula reveal an apparent paradox: while the frequency of synoptically forced dust storms has declined since the late 1990s, mean near-surface dust concentrations, poor-visibility events, and chronic air-quality degradation have increased. This contrast is often attributed to changes in emissions or land use. Here, we propose instead that the paradox reflects an abrupt dynamical regime shift in large-scale circulation and boundary-layer ventilation. The Arabian Peninsula is strongly influenced by baroclinic disturbances generated by short-wavelength Rossby waves radiated from the subtropical jet stream (STJ). These disturbances drive deep vertical coupling, strong surface winds, and efficient ventilation of the boundary layer. Multiple independent diagnostics indicate that the regional circulation underwent an abrupt transition in the late 1990s, marked by increased static stability, increased pressure depth of the troposphere, a reduction in the squared meridional temperature gradient, and a corresponding decline in mean available potential energy. These changes are consistent with weakened Rossby wave radiation and reduced baroclinic activity downstream of the STJ.

The consequences of this transition are twofold. First, reduced baroclinic activity suppresses deep convection, strong downdrafts, and synoptically driven high-wind events, leading to a decline in dust storm frequency. Second, and critically, weakened ageostrophic flow at the top of the boundary layer reduces shear-driven turbulence generation, particularly under stable boundary-layer conditions. The resulting collapse of vertical mixing limits ventilation and increases the residence time of dust near the surface, leading to higher mean surface concentrations despite fewer extreme dust events.

This framework extends a dynamical theory previously developed to explain abrupt increases in fog under weakened baroclinic forcing to mineral dust and air quality. The results demonstrate that reduced ventilation alone is sufficient to reconcile declining dust storm frequency with increasing surface dust loading, highlighting the nonlinear sensitivity of boundary-layer processes to large-scale circulation changes. The findings underscore the importance of regime shifts in atmospheric dynamics for understanding long-term changes in dust, pollution, and visibility in arid regions.

How to cite: Mhawish, A., Gunturu, U. B., Alamoudi, S., Alduaji, S., and Alqahtani, J.: Fewer Dust Storms, Greater Dust Concentration in the Air, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19014, https://doi.org/10.5194/egusphere-egu26-19014, 2026.

EGU26-19098 | ECS | PICO | AS3.5

Source-Limited Dust Emission in the Tarim Basin, China: Landform-Specific Parameterisation and Wind-Flux Hysteresis 

Yin Guo, Xin Gao, Jiaqiang Lei, and Wim Cornelis

Abstract: Dust emissions from the Tarim Basin, China, are governed by strong surface heterogeneity and finite sediment supply, two pivotal controls that can induce source depletion and wind-flux hysteresis during dust events. In this study, we adopt the source-limited dust emission (SLDE) scheme proposed by Shao (2025) and develop a landform-specific parameterization that couples remotely sensed surface units with field-measured particle-size data. Specifically, we generate a mutually exclusive seven-class geomorphology map in Google Earth Engine via a hierarchical decision tree, which integrates multi-source datasets including topography (MERIT DEM), vegetation coverage (MODIS NDVI), surface water occurrence (JRC Global Surface Water), and Sentinel-1 backscatter texture characteristics. The resultant geomorphological units comprise mobile dunes, vegetated hummock dunes, fixed/semi-fixed sandy lands, interdune areas, gobi/deflation surfaces, fluvial-lacustrine sediments, and mountain/loess terrains. For each unit, class-specific particle-size distributions are compiled from in-situ measurements and converted into discretized lookup tables, which serve as static input parameters for the SLDE scheme. Initial diagnostic experiments at both column and point scales, driven by hourly 10-m wind data from ERA5-Land (for the April 2020 case study), reveal distinct dust emission regimes across different landform types. On supply-limited surfaces-notably gobi/deflation and fluvial-lacustrine units-our simulations demonstrate that dust flux declines markedly under sustained high-wind conditions as the near-surface sediment reservoir becomes depleted, leading to pronounced hysteresis in the wind-flux relationship. The effective emission efficiency decreases from nearly unity at the onset of dust events to ~0.1 by the late stages, even when wind speeds remain above the threshold friction velocity for dust emission. In contrast, transport-limited behavior dominates in regions with ample sediment supply. These findings establish a physically interpretable framework for deriving SLDE parameters from geomorphological classifications and particle-size properties. Ongoing gridded simulations will quantify the extent to which sediment depletion reshapes the spatial contribution of key deflation zones, as well as the event-integrated dust emission budget, relative to results derived under conventional transport-limited assumptions.

Keywords: Source-limited dust emission; Source depletion; Wind-Flux Hysteresis; Particle size distribution

How to cite: Guo, Y., Gao, X., Lei, J., and Cornelis, W.: Source-Limited Dust Emission in the Tarim Basin, China: Landform-Specific Parameterisation and Wind-Flux Hysteresis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19098, https://doi.org/10.5194/egusphere-egu26-19098, 2026.

EGU26-19364 | ECS | PICO | AS3.5 | Highlight

Experimental Characterisation of the Electric and Magnetic Fields Generated by Dust Devils  

David Reid, Karen Aplin, and Nick Teanby

Lofted particulate in dust devils becomes charged through triboelectrification, that is, the exchange of charge in collision between grains. Electric fields from charged dust were first detected in the mid 17th century, with quantitative measurements recording in the region of kilovolts per metre. Magnetic field observations of dust devils are much less common, with the only published terrestrial measurement from 2001 in Arizona. The most complete magnetic field dataset associated with dust devils comes from NASA’s InSight mission to Mars, with 1200 sols of near-continuous observation, and over 15000 convective events detected, likely to be dust devils.  

To better understand the expected electric and magnetic fields generated by these aeolian features, a new apparatus was developed, building upon previous experimental work. The Terrestrial Experimental appaRatus for Investigating the Electric and magnetic fields of dust devils (TERIE) consists of a multi-instrumented 1000 mm diameter, 1200 mm tall tank, lined externally with grounded aluminium foil to act as a Faraday cage, and internally with sand to reduce the impact of tribocharging from particle-wall collisions. 

The apparatus records electric field strength at 4 vertical positions, and the (vector) magnetic field at 3 vertical positions. Through photodiodes, the optical thickness of the dust devil column can be evaluated, and offline sampling of the suspended particles can be used to understand the distribution through the profile of the simulated event. By incorporation of different mast positions, the radial profile of the generated field can also be investigated. 

Initial results from the new experimental apparatus show electric fields exceeding 40~kVm-1 were generated by the rotation of sand, with the distribution of the field broadly matching that expected from simulation. Some low frequency, sub-nanotesla variations in magnetic field were detected in the presence of rotating charged sand, consistent with expectations from models and previous experiments.  

How to cite: Reid, D., Aplin, K., and Teanby, N.: Experimental Characterisation of the Electric and Magnetic Fields Generated by Dust Devils , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19364, https://doi.org/10.5194/egusphere-egu26-19364, 2026.

EGU26-19688 | ECS | PICO | AS3.5

The Pb, Nd, and Sr isotopic characterisation of dust sources in North Africa and Western Asia. 

Daniel Howcroft, Anya Crocker, Rex Taylor, Agnes Michalik, J. Andy Milton, Nick Drake, Paul Breeze, Derek Keir, Michael Petraglia, Jaafar Jotheri, Deepak Jha, and Paul Wilson

Mineral dust is a key component of Earth’s climate system; it influences the global radiation budget, fertilises ecosystems, and constitutes a threat to human health. Accumulation of windblown dust in marine archives provides a means to assess past change in Earth’s continental hydroclimate. However, interpretations of these records are often undermined by an attribution problem: the uncertainty of provenance. Here we report new radiogenic isotope data (Sr, Nd, and Pb) from unconsolidated surface sediments sampled from active dust sources and integrate them with published geochemical and satellite-derived datasets (such as dust source activation frequency (DSAF)) to define preferential source areas (PSAs) across the Northern Hemisphere dust belt. Our analysis shows that pairing Pb with Nd or Sr isotope data allows clearer discrimination between source regions that overlap in Nd-Sr space. We also show that Pb data are particularly helpful to discriminate between sources when presented as D207Pb/204Pb and D208Pb/204Pb: deviations of Pb from the Northern Hemisphere Reference Line (NHRL) that defines the Pb isotopic evolution of the Northern Hemisphere’s mantle. Comparison with published Pb isotope data reveals major limitations in spatial coverage and suggests that application of more consistent cleaning protocols is merited including removal of anthropogenic Pb. Nevertheless, our new data help to discriminate among the dust sources of East Africa and Western Asia more clearly than before, improving our ability to interpret past continental hydroclimate change recorded in marine sediment cores from the northern Indian Ocean.

How to cite: Howcroft, D., Crocker, A., Taylor, R., Michalik, A., Milton, J. A., Drake, N., Breeze, P., Keir, D., Petraglia, M., Jotheri, J., Jha, D., and Wilson, P.: The Pb, Nd, and Sr isotopic characterisation of dust sources in North Africa and Western Asia., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19688, https://doi.org/10.5194/egusphere-egu26-19688, 2026.

EGU26-20205 | PICO | AS3.5

Selected Mineral Dust Events at the Sonnblick Observatory in 2024: Identification and Characterization Using In-Situ Data, PMF analysis and Atmospheric Transport Modelling 

Gerhard Schauer, Barbara Scherllin Pirscher, Alicja Skiba, Thomas Bachleitner, Kathrin Baumann-Stanzer, Anne Kasper-Giebl, and Julia Burkart

Mineral dust, emitted from soils in arid regions by wind erosion, represents one of the largest fractions of atmospheric aerosol by mass. Once airborne, dust can travel thousands of kilometers, influencing the atmosphere through scattering and absorption of sunlight, acting as ice-nucleating particles, and depositing on the ground where it reduces snow albedo and delivers nutrients to remote regions. High-altitude mountain stations provide a unique opportunity to study dust in the free troposphere and its long-range transport.

The Sonnblick Observatory (3106 m a.s.l.), located on the main ridge of the Austrian Alps, receives dust, particularly from Northern Africa, throughout the year. In this study, we focus on selected dust events during 2024, a year of particular interest due to one of the most intense events (aerosol mass above 700 µg/m3, 30 min averages) detected at the observatory. The observatory is a Global Atmosphere Watch (GAW) station, an Aerosol, Clouds, and Trace Gases Research Infrastructure (ACTRIS) aerosol in situ national facility and hosts a variety of aerosol, cloud and meteorological measurements.

Saharan dust events (SDEs) are initially identified using the “Saharan Dust Event Index,” routinely derived from in-situ optical measurements (nephelometer and aethalometer) at the station (Schauer et al. 2016). In addition, positive matrix factorization (PMF) of in-situ aerosol data is applied, with one significant factor interpreted as mineral dust and used for a second, independent event identification. PMF highlights events that may not be captured by the Saharan Dust Index, illustrating its potential as a complementary approach for dust detection. Individual events are further characterized using the full suite of in-situ measurements and weekly offline chemical composition analyses (inorganic ions, selected elements and carbohydrates as well as elemental and organic carbon) of PM10 filter samples, again combined with PMF analysis to identify major aerosol sources. Particle size distributions up to 100 µm during SDEs are retrieved from multiple instruments, including a mobility spectrometer, optical particle counter, and holographic measurements (SwisensPoleno Jupiter). Average size distributions are calculated for each event. Meteorological and atmospheric conditions are analyzed in relation to particle size distributions and optical properties. Particular attention is given to events identified solely by PMF.

Typical transport pathways are investigated using FLEXPART, and dust concentrations are simulated with WRF-Chem (Weather Research and Forecasting (WRF) model coupled with Chemistry) and compared with in-situ observations. The WRF-Chem simulation considers only dust emissions, generated by the AFWA (Air Force Weather Agency) dust emission scheme. Hourly-resolved surface dust concentration, vertically resolved dust concentration profiles, and dust load are available on a 0.2° x 0.2° latitude-longitude grid. The data also contribute to the Sand and Dust Storms Warning Advisory and Assessment System (SDS-WAS) model ensemble.

We summarize a full season of observed dust events, identify their characteristic features and develop a data analysis strategy applicable to longer time periods. In particular, we examine PMF analysis as a potential tool for SDE detection.

Schauer, G., Kasper-Giebl, A. and Mocnik, G. (2016); https://doi.org/10.4209/aaqr.2015.05.0337

Acknowledgements
The participation of A. Skiba was supported by the program “Excellence Initiative – Research University” for the AGH University of Krakow (ID:13958).

How to cite: Schauer, G., Scherllin Pirscher, B., Skiba, A., Bachleitner, T., Baumann-Stanzer, K., Kasper-Giebl, A., and Burkart, J.: Selected Mineral Dust Events at the Sonnblick Observatory in 2024: Identification and Characterization Using In-Situ Data, PMF analysis and Atmospheric Transport Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20205, https://doi.org/10.5194/egusphere-egu26-20205, 2026.

EGU26-21358 | PICO | AS3.5

The A-LIFE aircraft field experiment in the Eastern Mediterranean: what have we learned about mineral dust mixtures? 

Bernadett Weinzierl, Maximilian Dollner, Josef Gasteiger, Marilena Teri, Manuel Schöberl, Katharina Heimerl, Anne Tipka, Petra Seibert, Heidi Huntrieser, Robert Wagner, Konrad Kandler, Aryasree Sudharaj, Thomas Müller, Sophia Brilke, Nikolaus Fölker, Daniel Sauer, Oliver Reitebuch, Silke Groß, Volker Freudenthaler, and Carlos Toledano and the A-LIFE Science Team

Mineral dust is a key component of the globally-emitted aerosol mass. Although, mineral dust mixes with anthropogenic pollution during its atmospheric lifetime, data on polluted mineral dust layers have been scarce.

In April 2017, the A-LIFE aircraft field experiment (www.a-life.at) was carried out in the Eastern Mediterranean. A-LIFE combined ground-based, airborne, satellite, and modelling efforts to characterize mineral dust mixtures with unprecedented detail. In 22 research flights (~80 flight hours), outbreaks of Saharan and Arabian dust, as well as pollution, biomass burning, and dust-impacted clouds were studied, and a unique aerosol and cloud data set was collected. Aerosol source apportionment was achieved with the Lagrangian transport and dispersion model FLEXPART version 8.2. Based on FLEXPART model results and aerosol measurements, the observations were classified into 12 aerosol types consisting of four main aerosol types (Saharan dust, Arabian dust, mixtures with and without coarse mode). Each of the four main aerosol types was further separated into three sub-classes (clean, moderately-polluted and polluted). For each of the 12 aerosol classes, microphysical and optical aerosol properties were derived.

For the first time, the effect of pollution on the microphysical and optical properties of Saharan and Arabian dust was investigated systematically, revealing significant changes as a function of pollution content. The particle size distribution changes as a function of pollution content with effective diameters systematically decreasing for increasing pollution content. The collected data also provide new insights into the impact of Saharan and Arabian dust on cloud evolution processes, atmospheric radiation budget, and local meteorology. One outstanding finding of A-LIFE is that scattering properties of polluted dust mixtures do not show the typical dust signature, but rather show a wavelength-dependency of the scattering coefficient which is typical for pollution. This means that optical properties of mineral mixtures are frequently dominated by the pollution.

In this presentation, we will show the results of the A-LIFE project including its mission objectives, experimental design, and meteorological conditions; highlight major A-LIFE findings; and feature the available data products on the optical, microphysical, and hygroscopic properties of pure and polluted mineral dust.

How to cite: Weinzierl, B., Dollner, M., Gasteiger, J., Teri, M., Schöberl, M., Heimerl, K., Tipka, A., Seibert, P., Huntrieser, H., Wagner, R., Kandler, K., Sudharaj, A., Müller, T., Brilke, S., Fölker, N., Sauer, D., Reitebuch, O., Groß, S., Freudenthaler, V., and Toledano, C. and the A-LIFE Science Team: The A-LIFE aircraft field experiment in the Eastern Mediterranean: what have we learned about mineral dust mixtures?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21358, https://doi.org/10.5194/egusphere-egu26-21358, 2026.

EGU26-22343 | ECS | PICO | AS3.5

Sub-seasonal WRF-Chem reanalysis of extreme Saharan dust outbreaks in spring-summer 2024: balancing phase consistency and aerosol realism 

Alessandra Chiappini, Umberto Rizza, Giorgio Passerini, and Antonio Ricchi

Saharan dust outbreaks intermittently exert strong radiative, air quality and depositional impacts across the Euro-Mediterranean, due to the intrinsic characteristics of this phenomenon, yet their numerical reproduction remains challenging. Here we investigate modelling strategies that preserve spatio-temporal consistency in sub seasonal integrations with WRF-Chem, focusing on three major dust intrusions affecting Italy in 2024: 25 March to 1 April, 18 to 21 June, and 8 to 14 July. We perform a set of reanalysis driven experiments over a single 5 km grid domain spanning North Africa and the Mediterranean into continental Europe, forced by ECMWF IFS analyses at 6 hourly frequencies. Model performance is assessed against complementary observing systems over the Euro-Mediterranean with emphasis on Italy. Our core objective is to quantify how spectral nudging can mitigate large scale phase errors and long run drift, while avoiding an overly constrained mesoscale circulation that may distort dust emission, uplift and transport. In addition, using a sequence of sensitivity runs initialized at increasing lead times, we estimate event dependent spin-up thresholds that stabilize domain integrated dust mass and optical depth, while maintaining realistic emission timing, intensity and extension, to suggest a transferable good practice workflow for episodic dust reanalysis and for longer sub seasonal experiments. Overall, this study frames spectral nudging not as an arbitrary choice but as a tunable constraint whose optimal setting depends on the intended balance between large scale fidelity and internally generated aerosol meteorology feedback, with clear implications for WRF-Chem based dust assessments over Italy and the central western Mediterranean. The focus is on the fact that, despite an approximate 40% increase in computational time, the use of spectral nudging emerges as an optimized approach, both in terms of physical consistency and final computational cost savings. This technique proves particularly advantageous in reducing the overall number of simulations required within the context of sub-seasonal reanalysis.

How to cite: Chiappini, A., Rizza, U., Passerini, G., and Ricchi, A.: Sub-seasonal WRF-Chem reanalysis of extreme Saharan dust outbreaks in spring-summer 2024: balancing phase consistency and aerosol realism, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22343, https://doi.org/10.5194/egusphere-egu26-22343, 2026.

CR8 – Short Courses (SC) Education and Outreach Sessions (EOS)

EGU26-2979 | ECS | Posters on site | EOS1.4

Effects of emotional narratives and uncertainty visualization on non-experts’ trust in climate change forecast maps 

Sergio Fernando Bazzurri, Armand Kapaj, and Sara Irina Fabrikant

Climate change is an ongoing environmental and societal challenge. Communicating its ramifications and related uncertainties clearly to stakeholders and the public is an imperative task for time-critical decision-making. Public communication about climate change often includes maps, aimed at facilitating the understanding of complex scientific findings and making these more accessible to non-specialist audiences. This is especially important when difficult concepts such as inherent uncertainties related to climate predictions are involved.

While climate change communication may appear abstract and distant to non-experts, climate change discourse often involves strong emotional responses from the public. Engaging visual storytelling with climate change maps may be a useful strategy to reduce the psychological distance of the public. However, elicited emotions may influence how people perceive the presented information and thus their willingness to trust the maps.

We aimed to investigate the effect of emotional narratives on map readers’ trust in visualized (un)certainty information in static climate change forecast maps. We applied a 3x2 mixed factorial, map-based study design, including electrodermal activity measurements and eye-tracking. We designed three versions of climate change prediction map stimuli, inspired by the Swiss Climate Scenarios CH2018. Uncertainty was operationalized as a within-subjects independent variable such that participants viewed 18 map stimuli in total, showing different climate variables in randomized order, equally distributed across three conditions: (1) without uncertainty information, (2) uncertainty visualized as black gridded dots, or (3) uncertainty visualized as black randomly distributed dots. Following prior research, we used the term ‘certainty’ in our map stimuli, as it is better understood by the audience than ‘uncertainty’. We used narrative instructions as the between-subjects independent variable, with participants randomly assigned and matched across groups to one of the two conditions: (1) emotion or (2) control. In the emotion condition, each map stimulus was accompanied by an emotion-inducing verbal narrative and a human cartoon character. In the control condition, participants viewed the same map stimuli accompanied only by a factual verbal narrative.

We recruited 61 participants (30 females, 31 males, average age = 30 years) from the Department of Geography at the University of Zurich to participate in the study. After viewing each map stimulus, participants were asked (without any time restriction) to select one of the six predefined locations shown in the maps that they predicted to be most/least affected by climate change. Finally, they indicated their trust in each stimulus type using a standardized questionnaire.

Preliminary results suggest no significant differences in participants’ overall average trust ratings across the two narrative conditions. However, participants significantly trust climate change prediction maps more when certainty information is also included, regardless of the narrative condition they were assigned to. Conversely, we found no significant difference in trust ratings between the map stimuli that contain certainty information visualized as gridded or randomly distributed dots.

These novel empirical findings stress the need to visually communicate (un)certainty information to support people’s trust in climate science and climate change forecast maps. The use of cartoon characters to emotionally engage the public in climate change communication remains to be further empirically investigated.

How to cite: Bazzurri, S. F., Kapaj, A., and Fabrikant, S. I.: Effects of emotional narratives and uncertainty visualization on non-experts’ trust in climate change forecast maps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2979, https://doi.org/10.5194/egusphere-egu26-2979, 2026.

EGU26-5507 | ECS | Posters on site | EOS1.4

Communicating hydrological model calibration with toy examples 

Georgia Papacharalampous, Francesco Marra, Eleonora Dallan, and Marco Borga

Informing robust decisions on flood risk and water resource management necessitates, among other factors, clearer communication of hydrological model uncertainty to non-specialist audiences. In this presentation, we demonstrate that simplified toy models, which abstract away systemic complexity, can serve as an accessible and effective tool for this purpose. As a specific case study, we illustrate how the choice of calibration scoring function shapes model behavior and associated uncertainty estimates. This foundational approach helps build the core intuition needed to effectively engage with more complex, real-world systems. Overall, we present a practical framework that supports experts articulate, and non-experts comprehend, the essential "why" and "how" of uncertainty in hydrological predictions.

Acknowledgements: This work was funded by the Research Center on Climate Change Impacts - University of Padova, Rovigo Campus - supported by Fondazione Cassa di Risparmio di Padova e Rovigo.

How to cite: Papacharalampous, G., Marra, F., Dallan, E., and Borga, M.: Communicating hydrological model calibration with toy examples, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5507, https://doi.org/10.5194/egusphere-egu26-5507, 2026.

EGU26-7755 | Posters on site | EOS1.4

Making Sense of Uncertainties: Ask the Right Question 

Alexander Gruber, Claire Bulgin, Wouter Dorigo, Owen Emburry, Maud Formanek, Christopher Merchant, Jonathan Mittaz, Joaquín Muñoz-Sabater, Florian Pöppl, Adam Povey, and Wolfgang Wagner

It is well known that scientific data have uncertainties and that it is crucial to take these uncertainties into account in any decision making process. Nevertheless, despite data producer’s best efforts to provide complete and rigorous uncertainty estimates alongside their data, users commonly struggle to make sense of uncertainty information. This is because uncertainties are usually expressed as the statistical spread in the observations (for example, as random error standard deviation), which does not relate to the intended use of the data.

Put simply, data and their uncertainty are usually expressed as something like “x plus/minus y”, which does not answer the really important question: How much can I trust “x”, or any use of or decision based upon “x”? Consequently, uncertainties are often either ignored altogether and the data taken at face value, or interpreted by experts (or non-experts) heuristically to arrive at rather subjective, qualitative judgements of the confidence they can have in the data.

In line with existing practices (e.g., the communication of uncertianties in the IPCC reports), we conjecture that the key to enabling users to make sense of uncertainties is to represent them as the confidence one can have in whatever event one is interested in, given the available data and their uncertainty.

To that end, we propose a novel, generic framework that transforms common uncertaintiy representations (i.e., estimates of stochastic data properties, such as “the state of this variable is “x plus/minus y”) into more meaningful, actionable information that actually relate to their intended use, (i.e., statements such as “the data and their uncertainties suggest that we can be “z” % confident that…”). This is done by first formulating a meaningful question that links the available data to some events of interest, and then deriving quantiative estimates for the confidence in the occurrence of these events using Bayes theorem.

We demonstrate this framework using two case examples: (i) using satellte soil moisture retrievals and their uncertainty to derive how confident one can be in the presence and severity of a drought; and (ii) how ocean temperature analyses and their uncertainty can be used to determine how confident one can be that prevailing conditions are likely to cause coral bleaching. 

How to cite: Gruber, A., Bulgin, C., Dorigo, W., Emburry, O., Formanek, M., Merchant, C., Mittaz, J., Muñoz-Sabater, J., Pöppl, F., Povey, A., and Wagner, W.: Making Sense of Uncertainties: Ask the Right Question, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7755, https://doi.org/10.5194/egusphere-egu26-7755, 2026.

EGU26-11747 | ECS | Posters on site | EOS1.4

An overview of the scientific literature on uncertainty communication in geoscience  

Iris Schneider-Pérez, Marta López-Saavedra, Joan Martí, Judit Castellà, Solmaz Mohadjer, Michael Pelzer, and Peter Dietrich

Uncertainty is an inherent part of geoscience research and arises at multiple stages of the scientific process, from data collection and modelling to analysis and interpretation. In recent years, growing attention has been devoted to uncertainty quantification and assessment, alongside increasing recognition of the importance of uncertainty communication. These aspects are closely linked, as robust characterization of uncertainty provides an essential basis for transparent communication within the scientific community and beyond it.

Communicating uncertainty not only plays a key role in improving the understanding of how scientific knowledge is produced, but can also help to foster trust by increasing transparency and contextualizing results. Nevertheless, reluctance to explicitly assess and communicate uncertainty persists, particularly when addressing non-expert audiences. This challenge is especially relevant in the context of natural hazard risk assessment and management: Here, adequate communication of uncertainties can add particularly valuable information for decision-making, risk governance, and a better understanding of the risks at hand among public audiences.

This contribution presents an exploratory, database-driven overview of the scientific literature on uncertainty communication in geoscience, with a particular focus on natural hazards. Using structured queries in the Web of Science database, we examine publication trends over time, disciplinary distributions, thematic emphases, and possible blind spots. Keyword combinations range from general terms such as “uncertainty communication” and “multi-hazard communication” to more specific queries combining uncertainty, communication, and individual natural hazards (e.g., floods, earthquakes, droughts).

Preliminary results indicate that uncertainty communication spans a broad range of scientific categories, while the level of attention varies substantially across hazard types, with flood-related studies being more prominent than others. Initial findings also suggest that multi-hazard uncertainty communication remains comparatively underrepresented, despite the increasing emphasis on multi-hazard and multi-risk assessments in recent research and policy frameworks. The growing volume of publications further highlights the need for systematic approaches to literature mapping, as well as the potential role of data-driven and AI-assisted tools in supporting such analyses.

This research was partially funded by the European Civil Protection and Humanitarian Aid Operations (ECHO) of the European Commission (EC) through the VOLCAN project (ref. 101193100) and by the 2024 Research Prize of the Dr. K. H. Eberle Foundation to Mohadjer, Pelzer and Dietrich.

How to cite: Schneider-Pérez, I., López-Saavedra, M., Martí, J., Castellà, J., Mohadjer, S., Pelzer, M., and Dietrich, P.: An overview of the scientific literature on uncertainty communication in geoscience , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11747, https://doi.org/10.5194/egusphere-egu26-11747, 2026.

EGU26-11821 | Posters on site | EOS1.4 | Highlight

Heatwaves and Early Warning Systems: Perception Data and the Role of Science Communication – A Case Study from Romania 

Selvaggia Santin, Adina-Eliza Croitoru, Norbert Petrovici, Cristian Pop, Maria-Julia Petre, Enrico Scoccimarro, and Elena Xoplaki

Heatwaves are among the most impactful climate extremes in Europe, driving acute health risks and socio-economic disruption. They are a challenge for early warning and public understanding due to uncertainties in event onset, severity, and human response. Building on the interdisciplinary Strengthening the Research Capacities for Extreme Weather Events in Romania (SCEWERO) project funded by the European Union, this study investigates how scientific evidence, perception data, and communication strategies interact within Romania’s heatwave Early Warning System operated by Meteo-Romania. We analyse both empirical perception data — collected through structured surveys and focus groups to quantify how different communities interpret heat warnings, risk levels, and confidence intervals — and observational heatwave metrics to map divergences between communicated risk and public understanding. This research highlights specific sources of uncertainty faced by forecasters (e.g., variable heat exposure, model forecast spreads), and documents how these uncertainties are interpreted or misinterpreted by non-expert audiences. By tracing how uncertainty in forecast signals propagates through institutional warning messages and into public perception, we identify communication gaps that can lead to maladaptive responses or reduced trust in warnings during heat events. Framing uncertainty, contextualised risk information, and tailored communication strategies improve both public comprehension and behavioural intent during heatwave alerts. We propose evidence-based recommendations for operational Early Warning Systems that move beyond fixed deterministic thresholds, instead incorporating probabilistic messaging where appropriate and grounding risk communication in locally derived perception data. This work illustrates how harmonising scientific uncertainty communication with Early Warning practices can strengthen societal resilience to heatwaves, offering a transferable framework for climate risk communication in other European regions.

How to cite: Santin, S., Croitoru, A.-E., Petrovici, N., Pop, C., Petre, M.-J., Scoccimarro, E., and Xoplaki, E.: Heatwaves and Early Warning Systems: Perception Data and the Role of Science Communication – A Case Study from Romania, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11821, https://doi.org/10.5194/egusphere-egu26-11821, 2026.

Aquifer thermal energy storage (ATES) is a way to use the groundwater to heat and cool buildings, with very low CO2 emissions. It classifies as a shallow geothermal technology, and it is gaining popularity worldwide because of its sustainability, efficiency and cost-effectiveness. While its potential has been extensively proven in traditional homogenous, productive sandy groundwater layers, investing in more complex subsurface settings has greater financial risk. This is related to uncertainty about the (hydraulic) project feasibility and (thermal) efficiency of the system. Basically, we cannot directly look underground, so it is uncertain to what extent our subsurface model correctly represents reality. Even though this subsurface uncertainty leads to a great globally untapped potential for thermal energy storage, it is often neglected in feasibility studies. To move new ATES developments forward in complex subsurface settings, we present an uncertainty-driven sound scientific method to make investment decisions. Uncertainty in subsurface models is recognized by using a stochastic approach. The model predictions are then processed with clustering and global sensitivity analysis. This allowed to define criteria on critical subsurface properties that guarantee project (in)feasibility. For edge-cases, uncertainty is quantified to determine the probability of project feasibility from a risk-taking or risk-averse decision-maker perspective. Additionally, this approach quantified the potential of changing operational parameters (flow rate, well spacing, design injection temperature) to enhance project feasibility. All results are summarized in an easy-to-interpret decision tree that guides go/no-go decisions for new ATES projects. Importantly, the decision-tree can be followed prior to carrying out costly field tests. To illustrate, the uncertainty-driven decision tree approach is applied to a low-transmissivity aquifer for ATES, which represents a subsurface setting at the limit of ATES suitability. In conclusion, our approach effectively handles uncertainty while also focusing on improving clear communication to investors about the probability of project feasibility. As such, it could be an example study on how to handle model uncertainty for predictions of aquifer thermal energy storage systems in the future.

How to cite: Tas, L., Caers, J., and Hermans, T.: An Uncertainty-Driven Decision Tree Approach Guiding Feasibility Decisions of Shallow Geothermal Systems in Complex Subsurface Settings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14276, https://doi.org/10.5194/egusphere-egu26-14276, 2026.

EGU26-15153 | ECS | Posters on site | EOS1.4

Communicating Flood Risk Uncertainty for Decision-Making in Aotearoa-New Zealand 

Clevon Ash, Matthew Wilson, Carolynne Hultquist, and Iain White

Flood risk uncertainty is a growing problem in New Zealand and the rest of the world. Decision-makers are facing increasing uncertainty in planning for future events. Growing population centres, increased cost of living and the resulting increased exposure to these natural hazards are just some of factors they need to consider in planning and mitigating future events. Climate change predictions represent a large part of the uncertainty present in these future flood risk assessments. Variables such as rainfall intensity and duration are likely to change significantly with increased temperatures which would result in potentially larger and more frequent flood events. To better understand how these different uncertainties could influence decision-making, a series of flood model and risk assessment output representations containing uncertainty were generated from a Monte Carlo framework. These representations were tested using an online survey and focus groups across regional councils, national response agencies and private companies that work with flood information. The results showed that traditional flood outputs such as depth and extent were still rated more useful than uncertain outputs such as confidence and exceedance probabilities. Larger AEPs (annual exceedance probabilities) such as 0.5% and 0.1% were seen as useful for long-term development planning but lower AEPs such as 1% and 5% were better suited for mitigation and emergency response plans. Across all the uncertainty outputs, respondents stressed the need for additional contextual information such as socio-economic overlays, area specific information such as land use and building types that would work in tandem with rebuild cost estimates and building damage data. From this feedback, a series of recommendations for presenting flood uncertainty information to decision-makers were created.

How to cite: Ash, C., Wilson, M., Hultquist, C., and White, I.: Communicating Flood Risk Uncertainty for Decision-Making in Aotearoa-New Zealand, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15153, https://doi.org/10.5194/egusphere-egu26-15153, 2026.

EGU26-17550 | ECS | Posters on site | EOS1.4

Communicating the Uncertain Nature of Science Through the Lens of Science Education 

Jakub Stepanovic, Sandy Claes, and Jan Sermeus

Uncertainty is a defining feature of the nature of science; besides driving curiosity in research, its acknowledgement and reporting are expected to ensure transparency and credibility. However, when science is communicated to a non-expert audience, uncertainty often gets oversimplified or omitted. This practice can lead to misconceptions about science (e.g., science leads to absolute knowledge) or erode confidence when uncertainties inevitably surface. In this session, we will explore how uncertainty is framed within the Nature of Science framework of science education, and which educational strategies might be of interest for science communication. Drawing on examples from communicating planetary science, we will discuss approaches that can make uncertainty relatable and constructive, helping audiences appreciate science as a dynamic, evidence-based process rather than a collection of fixed facts.

How to cite: Stepanovic, J., Claes, S., and Sermeus, J.: Communicating the Uncertain Nature of Science Through the Lens of Science Education, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17550, https://doi.org/10.5194/egusphere-egu26-17550, 2026.

EGU26-20429 | ECS | Posters on site | EOS1.4

Communicating uncertain future climate risk: Lessons learned from adaptation and disaster risk practitioners in Madagascar 

Ailish Craig, Rachel James, Alan Kennedy-Asser, Elisabeth Stephens, Katharine Vincent, Richard Jones, Andrea Taylor, Christopher Jack, Alice McClure, and Christopher Shaw

Climate information is increasingly being produced and shared as governments, businesses and individuals need to adapt to the changing climate. Yet, communicating uncertain climate change information to non-experts remains a challenge. The information that is currently made available to non-climate science specialists is too complex for them to understand and use. A key challenge in climate science is that estimating future change comes with uncertainties which are highly technical to non-climate specialists. Nevertheless, it is paramount that when climate information is shared and used, the limitations and uncertainties attached are well understood. This is particularly important amongst audiences that lack technical familiarity with climate science. Additionally, scientists and climate service providers do not have a common approach to represent the range of future change. Some scientists place an emphasis on probabilistic projections, meanwhile others focus on the full range of plausible futures.

There has been a limited effort to assess whether the audience understands what the producer of the climate information intended. Testing or evaluating different methods and visualisations of communicating future climate information, and its related uncertainties, can provide insight into what is most effective. Isolating what is (mis)understood can shed light on how to effectively communicate future climate information. This study investigates the interpretation of different presentations of future climate information using a survey and discussion with 45 participants working within weather and disaster agencies in Madagascar. Icon arrays, climate risk narratives, key statements and verbal probability language was tested to provide insight into how practitioners understand different ways of communicating future climate information. Both probabilistic and plausible framings of uncertainty are considered to explore how participants interpret each.

The percentage of participants that selected the correct answers across comprehension questions ranged from 24-82%. For the interpretation of verbal and numeric probabilities which was communicated as “virtually certain [99-100%]”, the correct numerical probability was selected by 24% of participants, highlighting the systematic misinterpretation of verbal and numerical probabilities. The climate risk narrative provided 3 plausible narratives, however, over a third of participants incorrectly believed there were 3 narratives to allow decision makers to select a narrative that is sector relevant. Some reasons for misinterpretation were provided by the participants such as confusing legends and icons, using their prior knowledge instead of the information document or experiencing cognitive dissonance. Meanwhile some expressed difficulty understanding due to lots of information while others requested additional insights, demonstrating the need for flexibility in design.

This study has highlighted new ways of communicating climate risk as well as ineffective current practises.  Recommendations suggest that climate scientists and climate communicators should; include an explicit explanation of why there are multiple climate risk narratives; reconsider the use of numeric and verbal probability expression given they are commonly misinterpreted and consider that an individuals’ prior knowledge influences their interpretation of new information. 

How to cite: Craig, A., James, R., Kennedy-Asser, A., Stephens, E., Vincent, K., Jones, R., Taylor, A., Jack, C., McClure, A., and Shaw, C.: Communicating uncertain future climate risk: Lessons learned from adaptation and disaster risk practitioners in Madagascar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20429, https://doi.org/10.5194/egusphere-egu26-20429, 2026.

EGU26-44 | ECS | Orals | EOS1.1

SmarTerrae: Applied scientific training in geoscience from the earliest educational stages 

Lorena Salgado and Rubén Forján

We present an educational, learn-by-doing model that integrates real-world projects in geosciences, environmental management and conservation with the production and active dissemination of scientific outputs, complemented by digital communication as a largely passive outreach channel. The programme is motivated by a pronounced disconnection among young people—including those enrolled in environmental and territorial studies—and the place-based problems that surround them, a gap that jeopardizes the near-term availability of qualified environmental and land-management professionals. Our objective is to engage secondary, baccalaureate, vocational (FP), and undergraduate students as active participants in problem identification, project co-design, and execution—equipping them with the conceptual and technical tools needed to address environmental and territorial challenges in the north-west of the Iberian Peninsula.

A quasi-experimental pre-test–post-test design without a control group was implemented across multiple educational levels. The evolution of perceptions and competences was assessed using Likert-scale questionnaires, a register of scientific outputs, and baseline Instagram analytics. A distinctive feature of the model is that students are not only active co-designers of each project but also the primary executors of fieldwork and analysis under light supervision. In addition, they regularly present in age-appropriate scientific fora (e.g., school symposia, regional conferences), which deepens their sense of ownership and strengthens the bond with both the project and the territory.

Results indicate general improvements in interest in science and the environment, data-analysis capability, understanding of the research process, and willingness to participate in scientific activities. Tangible, transferable outputs were generated (e.g., a conference poster and articles published or in preparation), and continuity of training pathways was established. The @SmarTerrae profile is consolidating as a knowledge-transfer channel during the programme’s implementation phase, complementing in-person dissemination.

How to cite: Salgado, L. and Forján, R.: SmarTerrae: Applied scientific training in geoscience from the earliest educational stages, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-44, https://doi.org/10.5194/egusphere-egu26-44, 2026.

EGU26-712 | Posters on site | EOS1.1

Evaluating Dendroclimatology-Based Climate Education Across Stakeholder Groups in the Ukrainian Carpathians 

Dariia Kholiavchuk, Jan Šebesta, Maryna Dranichenko, Vladyslav Maievskyi, Alina Horiuk, Karolina Shestobanska, Yuliia Kuzenko, and Serhii Tokariuk

Translating paleoclimate evidence into actionable climate literacy requires context-specific pedagogical approaches. This study evaluates whether tangible proxy data (tree-ring records) enhances climate change comprehension compared to abstract datasets. It assesses differential educational strategies for three stakeholder groups with varying knowledge bases and decision-making responsibilities.

We conducted structured field workshops with 52 participants across three cohorts in the Ukrainian Carpathians during 2025 as part of the “Capacity Building for Research and Protection of Natural Forests in Western Ukraine” project. In collaboration with the Chernivtsi City Council’s Climate Policy Division, we designed learning objectives aligned with municipal adaptation planning needs, addressing a critical gap where protected area managers lack access to climate education. This integration of local ecological data with regional adaptation frameworks aims to enhance the effectiveness of climate adaptation efforts. University academics (n=8) and protected area rangers (n=4) attended seven-day workshops at Carpathian Biosphere Reserve and Vyzhnytskyi National Natural Park (July 2025). A separate field seminar at Tsetsyno highland employed a cascading pedagogy, where trained third-year geography students (n = 7) facilitated learning for second-year students (n = 7) and secondary pupils (grades 9-12, n = 25) in October 2025. All participants completed pre-workshop climate knowledge assessments, post-workshop evaluations, and structured feedback surveys (100% response rate).

Standardised content included physical examination of increment cores from 50- to 200-year-old beech and spruce, interpretation of ring-width chronologies showing documented climate extremes (the 1990s warming and the 2003 heatwave), soil and vegetation analysis, and regional temperature reconstruction visualisation (1750-2024). Municipal climate policy staff co-designed ranger modules emphasising management applications, including translating paleoclimate uncertainty into risk assessment and developing evidence-based adaptation strategies. Pre-assessment revealed critical baseline differences. Academics demonstrated strong theoretical knowledge (mean: 78%) but limited practical application capacity. Rangers possessed detailed, contemporary observational knowledge (mean: 65%), but lacked a historical context of climate. 93% of them could not identify whether current warming rates were unprecedented regionally. Secondary students showed the lowest baseline comprehension (mean: 41%).

Post-workshop assessments revealed differential gains among the groups. Rangers demonstrated the most significant increase in knowledge, particularly in interpreting timescales of climate variability. Academics showed modest gains, primarily in translating research for non-specialist audiences. Student moderators achieved substantial gains through the dual benefits of content mastery and pedagogical skill development. Secondary students showed significant improvements, with hands-on “tree doctor” activities generating the strongest engagement. Tangible proxy data effectively addressed the challenges of abstract temporal scales. Local site selection proved critical as participants connected evidence directly to familiar landscapes and management contexts.

Small sample sizes limit the generalizability of the findings, which represent a proof-of-concept that requires validation through larger studies and a cost-effectiveness analysis. However, the results suggest that paleoclimate proxies effectively communicate climate context to decision-makers who lack historical baselines, which is a critical gap in adaptation planning. The research-governance partnership model demonstrates how academic institutions can support the implementation of municipal climate policies through targeted capacity building, resulting in measurable outcomes in resource management and education.

How to cite: Kholiavchuk, D., Šebesta, J., Dranichenko, M., Maievskyi, V., Horiuk, A., Shestobanska, K., Kuzenko, Y., and Tokariuk, S.: Evaluating Dendroclimatology-Based Climate Education Across Stakeholder Groups in the Ukrainian Carpathians, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-712, https://doi.org/10.5194/egusphere-egu26-712, 2026.

EGU26-800 | ECS | Orals | EOS1.1

Speculative Storytelling as a Tool for Biodiversity and Climate Communication 

Chiara Anzolini, Fabio De Pascale, and Telmo Pievani

Communicating biodiversity loss and climate disruption to non-specialist audiences requires approaches that translate complex scientific processes into accessible and emotionally resonant forms. Speculative storytelling, including science fiction and future-oriented narratives, offers a promising strategy. By imagining plausible futures grounded in current scientific knowledge, these narratives illuminate the consequences of environmental change while encouraging reflection on societal choices, adaptive behaviours, and potential pathways forward.
Within the Science and Society spoke of the National Biodiversity Future Center (NBFC), funded by Italy’s National Recovery and Resilience Plan (PNRR), we adopt an interdisciplinary, research-informed framework for the design of such narratives. Science communicators operate as intermediaries between researchers and creative professionals – writers, illustrators, media producers – ensuring both scientific accuracy and narrative coherence. This role includes conceptual development, the selection of scientific experts based on thematic relevance and communication skills, and continuous collaboration throughout the creative process. It also extends to the public-facing dissemination of the resulting works, enabling coherence between scientific objectives, artistic expression, and audience engagement.

A key aspect of this approach is the strategic use of distinct speculative modes to engage different audiences. Dystopian narratives explore the ecological and social implications of biodiversity loss by depicting futures in which degraded ecosystems or climate-altered conditions shape daily life, effectively highlighting risks and long-term consequences. In contrast, positive or “post-crisis” futures imagine societies that have adopted sustainable practices and redefined their relationship with natural systems, promoting a sense of agency and motivating constructive engagement.
Embedding rigorous scientific input within imaginative world-building allows speculative storytelling to convey biodiversity and climate issues in ways that extend beyond traditional educational formats. By making abstract temporal scales, uncertain projections, and complex socio-ecological dynamics more concrete, these narratives support both understanding and emotional resonance. The use of varied media – from comics to podcasts – further enables the tailoring of content to diverse publics and communication contexts.
I will discuss selected initiatives that employ speculative storytelling for biodiversity and climate communication across different media formats. These examples show how interdisciplinary, narrative-driven approaches can create science communication that is both emotionally engaging and scientifically robust, enriching public understanding of environmental change.

How to cite: Anzolini, C., De Pascale, F., and Pievani, T.: Speculative Storytelling as a Tool for Biodiversity and Climate Communication, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-800, https://doi.org/10.5194/egusphere-egu26-800, 2026.

The project ‘Prison talks: bringing climate change conversations into the Irish prisons’ has been awarded an EGU Public Engagement Grant. This public engagement project brings talks on climate change, extreme weather events, and their impacts to inmates (people in prison) in Irish prisons, through the lens of science communication and outreach.

This project is raising awareness of climate change and its impacts among people in prison, a hard-to-reach audience with limited access to science communication and outreach activities. People in prison have an educational disadvantage, as many didn’t finish secondary school. This climate change outreach project plays a transformative role by providing values, knowledge, and skills to help individuals reach their full potential, motivate positive citizenship, develop social responsibility and personal transformation, increase well-being, and foster a sense of community and belonging, enabling them to live more successfully upon release.

People in prison completed anonymous surveys (quantitative and qualitative questions) before and after attending the climate change talks to assess their perceptions of climate change and science communication and to evaluate the project's effectiveness.

This presentation will outline the research methods, lesson plans, project’s findings and recommendations. The project ‘Prison talks: bringing climate change conversation into the Irish prisons’ highlights awareness of the importance of science communication and public engagement events among populations in prisons, which can be replicated in other countries.

How to cite: Mateus, C.: Prison talks: bringing climate change conversations into the Irish prisons, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-853, https://doi.org/10.5194/egusphere-egu26-853, 2026.

EGU26-1010 | ECS | Orals | EOS1.1

From Science to Practice: Co-Designing Windstorm Hazard & Risk Information for Dutch Portals 

Maria del Socorro Fonseca Cerda, Hans de Moel, Jeroen Aerts, Wouter Botzen, Koen Veenenbos, Lars de Ruig, Lisette Klok, and Toon Haer

Extreme winter windstorms are among the most expensive natural disasters in Europe and pose significant social and economic challenges.  The Netherlands frequently experiences winter storms that result in serious damage and large financial losses, especially for sectors like infrastructure and the built environment.

Climate Adaptation Services (CAS) created and manages national climate risk portals, such as the Klimaateffectatlas (www.klimaateffectatlas.nl) and the newly launched Dutch Climate Risk Portal (www.dutchclimaterisk.nl), which have helped the public in understanding vulnerabilities and risks by providing information on floods, drought, heat, and water-related hazards. However, until 2025, windstorms remained an essential missing risk, limiting urban and financial stakeholders' ability to interpret exposure and losses to these storms.

We studied winter windstorms, creating hazard maps and risk estimates. However, these scientific outputs are not directly applicable or understandable to stakeholders with diverse backgrounds and needs. Therefore, in collaboration with CAS, we co-created a map narrative and risk estimation tool, which was created through an iterative cycle of stakeholder workshops, feedback, and narrative design. The process aimed to make complex risk information accessible, usable, and intuitively understood for a wide range of users, regardless of technical background. The end result is the translation of windstorm science into practice, which is publicly available at the Klimaateffectatlas and the Dutch Climate Risk Portal, while ensuring relevance, clarity, and real-world impact for decision-makers.

How to cite: Fonseca Cerda, M. S., de Moel, H., Aerts, J., Botzen, W., Veenenbos, K., de Ruig, L., Klok, L., and Haer, T.: From Science to Practice: Co-Designing Windstorm Hazard & Risk Information for Dutch Portals, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1010, https://doi.org/10.5194/egusphere-egu26-1010, 2026.

EGU26-1385 | Orals | EOS1.1

Scientific Storytelling in Geodesy: Using Cartoons, Videos, and Digital Platforms to Reach New Audiences 

Martin Sehnal, Laura Sánchez, and Detlef Angermann

Geodesy plays a fundamental role in observing and understanding Earth system processes, yet its societal relevance often remains under-recognized outside the specialist community. To address this gap, the Global Geodetic Observing System (GGOS) of the International Association of Geodesy (IAG) has expanded its science communication activities during the recent years to make geodetic concepts, products, and techniques accessible to diverse audiences. This contribution presents an integrated communication strategy combining digital platforms, visual storytelling, and community-driven initiatives.

A central element is the renewed GGOS and IAG web platform https://geodesy.science, which provides an easy understandable introduction to geodesy as well as clear, non-technical explanations of observation techniques, products, and real-world applications.

Complementing this, a growing series of multilingual short films (https://www.youtube.com/@iag-ggos) communicates the importance of geodesy for monitoring climate change, natural hazards, sea-level rise, and global reference frames. These videos have reached broad international audiences and are frequently used in public outreach events such as open-day exhibitions.

The newest initiative is the Geodesy Cartoons project https://geodesy.science/cartoon , which communicates complex geodetic topics through approachable, story-driven visual narratives. The associated Geodesy Cartoon Competition actively involves the international geodetic community in co-creating educational illustrations. This participatory approach fosters shared ownership, stimulates creativity, and supports the development of communication material usable across research, teaching, and outreach.

Together, these multimedia tools illustrate how geodesy contributes to society’s daily life and decision-making. This presentation reflects on successes and challenges in designing accessible content, coordinating contributions across the global geodesy community, and evaluating engagement through online analytics and feedback. By sharing insights from these ongoing initiatives, we aim to contribute to a broader discussion on effective communication of Earth and space sciences and to strengthen connections between geodesy and the wider public.

How to cite: Sehnal, M., Sánchez, L., and Angermann, D.: Scientific Storytelling in Geodesy: Using Cartoons, Videos, and Digital Platforms to Reach New Audiences, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1385, https://doi.org/10.5194/egusphere-egu26-1385, 2026.

EGU26-1611 | Posters on site | EOS1.1

Innovative Tools for Science Education: Classroom Materials and Games from the INSE Project 

Eva Feldbacher, Laura Coulson, Carmen Sippl, Babette Lughammer, Ioana Capatu, Gregor Jöstl, Dominik Eibl, Michaela Panzenböck, Clara Rosenberger, Aimie Jung, and Gabriele Weigelhofer

The INSE project (Interdisciplinary Network for Science Education, led by WasserCluster Lunz and funded by GFF NÖ) has developed a comprehensive set of innovative, classroom-ready materials designed to strengthen scientific literacy across all educational levels. Co-created by researchers from the natural, social, and educational sciences together with partner schools, the materials translate core principles of scientific inquiry into engaging, age-appropriate learning experiences. All resources are freely available online and have been successfully tested in classroom settings.

For the primary level, the module The Forest of the Future introduces humanities-based inquiry through storytelling, exploratory learning, and creative techniques. Children investigate questions about environmental futures by engaging in narrative-based research tasks, learning how observation, interpretation, and imagination contribute to knowledge creation.

At the lower secondary level, a set of interactive Nature of Science (NOS) materials helps students understand the characteristics of scientific thinking. Activities highlight scientific evidence, uncertainty, the iterative nature of research, and the diversity of scientific methods. Abstract NOS concepts become tangible through hands-on tasks, role-play activities, and small-scale investigations.

For the upper secondary level, two modules allow students to conduct their own research:
(1) a natural science module in which students design and conduct an aquatic ecology respiration experiment, learning to formulate hypotheses, plan experiments, collect data, and interpret results; and
(2) a social science module that introduces learners to empirical social research through survey projects. Both modules guide students through the full research cycle and encourage reflective, evidence-informed thinking.

Beyond these core teaching packages, the project developed additional tools that make scientific inquiry accessible across informal and formal learning contexts: The research quartet Go Science introduces children aged 8+ to the fundamental steps of scientific inquiry through a playful card game. For teenagers, the Dive into Science learning app offers an interactive experience in which learners navigate scientific decisions based on real research questions - selecting hypotheses, designing experiments, analyzing sample datasets, and receiving direct feedback. Complementing these tools, the SCIBORG science board game supports learners aged 16+ in deepening their understanding of the scientific process.

Together, the INSE materials provide a powerful set of educational tools for fostering curiosity, critical thinking, scientific literacy, and trust in research. By showing how science works in practice, they support educators in integrating authentic scientific inquiry into everyday teaching.

In this presentation, we will showcase the full range of materials, allowing participants to explore, try out, and interact with the resources directly.

How to cite: Feldbacher, E., Coulson, L., Sippl, C., Lughammer, B., Capatu, I., Jöstl, G., Eibl, D., Panzenböck, M., Rosenberger, C., Jung, A., and Weigelhofer, G.: Innovative Tools for Science Education: Classroom Materials and Games from the INSE Project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1611, https://doi.org/10.5194/egusphere-egu26-1611, 2026.

EGU26-1677 | Posters on site | EOS1.1

Integrating Science Communication into Spain’s Atmospheric products: Insights from RESPIRE and CAMS-NCP 

Karinna Matozinhos de Faria, Marc Guevara, Paula Castesana, Paula Camps, Ivan Lombardich, Oliver Legarreta, Antonia Frangeskou, Diana Urquiza, Carles Tena, Francesco Benincasa, Elliott Steven, Santiago Ramírez, Carlos Pérez García-Pando, Yolanda Luna, Ernesto Barrera, Omaira Elena Garcia Rodriguez, and Ruben del Campo

Effective science communication is a central component of two major atmospheric initiatives in Spain: the “high-Resolution air Emissions Systems to suPport modellIng and monitoRing Efforts” (RESPIRE) and the Spanish component of the Copernicus Atmosphere Monitoring Service – National Collaboration Programme (CAMS-NCP). Both efforts, led collaboratively by the Barcelona Supercomputing Center (BSC) and the Spanish Meteorological Agency (AEMET), demonstrate how communication can be embedded into the design, implementation and societal uptake of advanced environmental projects.

Within RESPIRE, communication is treated as a strategic pillar supporting the development of high-resolution emissions estimates for air quality modelling and greenhouse gas (GHG) monitoring in Spain. Activities range from intuitive digital interfaces and stakeholder workshops to targeted web updates, newsletters, and social media outreach. A central element is a user-centric web application that visualizes carbon dioxide (CO₂) and methane (CH₄) fluxes. Together, these channels translate complex modelling outputs into actionable knowledge for public administrations, scientists, the private sector and citizens.

The CAMS-NCP communication strategy complements this by strengthening the visibility, understanding and uptake of CAMS products across national, regional and local levels. Building on the user network established during the first phase of the programme, Phase 2 implements a structured Communication and User Outreach Plan targeting policymakers, researchers, air quality planners, NGOs and citizens. Communication actions include regular updates to the CAMS-NCP website, coordinated press and social media campaigns, annual use case publications, and participation in national scientific and environmental events. Three annual CAMS User Forums and a final dissemination event provide spaces for technical dialogue, co-design and user feedback.

Across both initiatives, long-term communication experience reveals consistent lessons. Iterative co-creation with users increases uptake and ensures that tools respond to real needs. Trust is fostered through transparent messaging that acknowledges uncertainties while demonstrating methodological robustness. Effective communication requires not oversimplification but a strategic tailoring of information to specific decision contexts, from policy design and mitigation tracking to public awareness.

The challenges faced are also shared: conveying technically dense atmospheric information to non-experts, managing expectations about product capabilities, and maintaining visibility amid numerous parallel initiatives. Despite this, successes are significant. RESPIRE- has received international recognition from the Integrated Global Greenhouse Gas Information System (IG3IS), an initiative of the World Meteorological Organization (WMO), while CAMS-NCP continues to expand its user community and reinforce national alignment with European atmospheric services.

Together, RESPIRE and CAMS-NCP show how integrating communication into environmental science projects enhances societal impact. By combining advanced modelling with intentional, user-focused communication, both initiatives contribute to a more informed society and strengthen Spain’s capacity to address climate change and air quality challenges.


 

 


 

How to cite: Matozinhos de Faria, K., Guevara, M., Castesana, P., Camps, P., Lombardich, I., Legarreta, O., Frangeskou, A., Urquiza, D., Tena, C., Benincasa, F., Steven, E., Ramírez, S., Pérez García-Pando, C., Luna, Y., Barrera, E., Elena Garcia Rodriguez, O., and del Campo, R.: Integrating Science Communication into Spain’s Atmospheric products: Insights from RESPIRE and CAMS-NCP, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1677, https://doi.org/10.5194/egusphere-egu26-1677, 2026.

EGU26-1870 | Orals | EOS1.1

Interactive wetland education: Classroom materials following a constructivist instructional framework (Horizon Europe Restore4Life) 

Gabriele Weigelhofer, Tim Grandjean, Eva Feldbacher, Clara Rosenberger, Viktória Miklósová, Alma Mikuška, Dubravka Čerba, Jasna Grabić, Zorica Srđević, and Gabriela Costea

Wetlands are some of the most endangered ecosystems on the planet. There is an urgent need for large-scale wetland restoration and protection efforts that involve local community support. In our Horizon Europe project, Restore4Life (https://restore4life.eu/citizen-science/), we have developed a range of innovative offline and online educational materials to raise awareness of the vital ecosystem services that wetlands provide to humans.

Our materials are based on the 5E constructivist learning model. This inquiry-based, student-centered approach encourages active learning as students’ knowledge is built on understanding connections and processes. The five phases start with capturing students' interest and assessing prior knowledge/misconceptions (Engage), leading to investigating topics through hands-on activities and observations (Explore). In the Explain phase, students interpret their findings with the teacher's support. The last two phases focus on the application of the students’ newly acquired knowledge to deepen their understanding (Elaborate) and, finally, on the knowledge assessment by students and teachers (Evaluate). While our materials were developed for 12-14-year-olds, they can be easily adapted to younger or older kids.

Beyond these core teaching packages, the project developed additional tools, such as the “Blue-Green Space4All” game, a dynamic Wetland Fresk, available in both online and offline formats. A manual and a video provide instructions for building a simple treatment wetland, and our Wetland4Life App can be used to assess the wetland status directly in the field. All resources are freely available online (Zenodo) and have been successfully tested in classroom settings. Together, the Restore4Life materials provide a robust set of educational tools for fostering understanding of the significance of intact wetlands for human well-being.

In this presentation, we will showcase 5E teaching materials on the social, economic, and ecological benefits of intact wetlands, including supplying construction materials, providing recreational areas, and mitigating climate change and pollution. Participants can explore, test, and interact with the materials. Restore4Life is funded by the European Union.

How to cite: Weigelhofer, G., Grandjean, T., Feldbacher, E., Rosenberger, C., Miklósová, V., Mikuška, A., Čerba, D., Grabić, J., Srđević, Z., and Costea, G.: Interactive wetland education: Classroom materials following a constructivist instructional framework (Horizon Europe Restore4Life), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1870, https://doi.org/10.5194/egusphere-egu26-1870, 2026.

EGU26-1949 | Orals | EOS1.1

A little bit of activism increases trust in climate scientists 

Erik van Sebille, Celine Weel, Rens Vliegenthart, and Mark Bos

Some climate scientists refrain from advocacy and activism in their science communication because they fear it decreases their credibility. But whether there is indeed a relation between activism and credibility can be tested.

Here, we discuss the results of an experiment where 1,000 Dutch respondents first read a text on the impacts of the greening of gardens. Respondents are randomly assigned to either a version written in neutral tone, or a version written in an advocating tone. We then compare how the respondents perceive the credibility of the authoring scientist in these texts.

Our analyses show that the perceived credibility of the scientist who authored the text increases by advocacy overall, and that the advocating scientist is considered more credible than the neutral scientist specifically in their perceived sensitivity and care for society.

Based on these results, we conclude that advocacy can increase the climate scientist's average perceived credibility. This study may thus serve as endorsement for the many climate scientists who are willing to take a more advocacy-driven approach in their communications but are unsure of the consequences.

How to cite: van Sebille, E., Weel, C., Vliegenthart, R., and Bos, M.: A little bit of activism increases trust in climate scientists, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1949, https://doi.org/10.5194/egusphere-egu26-1949, 2026.

It has been well documented that social norms play a key role in motivating behavioral change. Although research on the effects of normative messages on pro-environmental decision-making has increased in recent years, our understanding of how these messages influence behavior remains limited (Chung & Lapinski, 2024). In particular, many pro-environmental behaviors have not yet achieved widespread adoption, and normative influences are often ineffective in such contexts. Consequently, scholars have begun to focus on dynamic norms, which refer to changing patterns of norms surrounding specific behaviors (Sparkman & Walton, 2017). When only a minority engages in a particular behavior, static norms that reflect behavior at a single point in time may inadvertently discourage action by emphasizing low participation rates. In contrast, dynamic norms, which highlight increasing popularity of a given behavior, have been shown to promote engagement (Sparkman & Walton, 2017). Accordingly, dynamic norms are considered particularly effective in contexts where pro-environmental behaviors have not yet become the majority practice. However, empirical evidence remains limited, and existing findings are inconsistent.

To advance understanding of norm framing effects (static vs. dynamic), the present study examines the underlying mechanisms through which norm framing influences behavior and investigates how these effects vary as a function of individual skepticism, specifically in the context of climate change. Environmental skepticism—defined as the tendency to doubt the seriousness, causes, or scientific evidence of environmental problems—has been identified as a key factor hindering effective environmental communication and behavior change.

An online experiment was conducted with 367 participants in South Korea. Participants first completed measures assessing climate change skepticism and were then randomly assigned to one of two norm-framing conditions (static vs. dynamic) related to pro-environmental behaviors aimed at mitigating climate change. They subsequently responded to measures of key variables.

The results indicated that the interaction between norm framing and skepticism did not significantly affect preconformity; however, it had a significant effect on reactance. Specifically, higher levels of skepticism were associated with greater reactance in response to dynamic norm messages compared to static norm messages. Moreover, this increased reactance was associated with reduced pro-environmental attitudes and behavioral intentions. This study contributes to the theoretical understanding of normative influence and climate change skepticism and offers practical implications for climate communication as well as directions for future research.

 

References

Chung, M., & Lapinski, M. K. (2024). The effect of dynamic norms messages and group identity on pro-environmental behaviors. Communication Research, 51(4), 439–462.

Sparkman, G., & Walton, G. M. (2017). Dynamic norms promote sustainable behavior, even if it is counternormative. Psychological Science, 28(11), 1663–1674.

How to cite: Kim, J. and Shin, G.: Normative Influences and Climate Change Mitigation: How Skeptical Individuals Respond to Dynamic Norm Messages and Why, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2148, https://doi.org/10.5194/egusphere-egu26-2148, 2026.

EGU26-2340 | Posters on site | EOS1.1

Expanding remote sensing–based environmental education: the Ecoview competition from national to international level 

Svitlana Babiichuk, Stanislav Dovgyi, and Lidiia Davybida

The rapid development of Earth observation technologies presents significant opportunities to promote environmental responsibility and data literacy globally. Building on the success of the All-Ukrainian competition "Ekopohliad" ("Ecoview"), established in 2019 by the GIS and Remote Sensing Laboratory of the National Centre "Junior Academy of Sciences of Ukraine", the initiative was expanded internationally in 2024 and 2025. The International Ecoview competition aims to engage school students (14-18 years old) from different countries in investigating real environmental and climate-related problems using open satellite data and geospatial tools. Participation requires the use of open-access remote sensing datasets and their analysis through accessible platforms, such as Copernicus Browser, Google Earth Engine, NASA Giovanni, NASA Worldview, Google Earth Pro, and QGIS.

The competition combines independent student research, mentor guidance, and evaluation by an international jury of experts in Earth observation and environmental science. Educational support includes webinars, methodological guidelines, and a video course on satellite data and GIS analysis, ensuring students develop practical research and analytical competencies. 

The first international edition in 2024 engaged 96 students from all school grades (K–12) from Ukraine and 14 other countries. In 2025, the competition was limited to participants aged 14–18 years to ensure fair competition among students of comparable age, engaging 60 students from Ukraine and 16 foreign countries, with balanced representation from Europe, Asia, Africa, and Latin America. Twenty finalists presented research covering a wide range of environmental topics, including urban environments, forests, surface water, desertification, extreme events, climate change, and notably, the ecological consequences of war. The diversity of geographical contexts allowed participants to compare environmental processes across regions and to develop a broader understanding of global environmental challenges.

Preliminary outcomes indicate that the international format of Ecoview enhances students' motivation, promotes critical thinking, and improves their ability to work with primary geospatial data sources. The competition also contributes to the formation of an international youth community interested in applying remote sensing for environmental research and sustainable development. These positive results demonstrate the project's effectiveness and underscore the need for continued support and expansion of the initiative.

Future priorities include expanding participation, strengthening the educational component with updated materials, promoting interdisciplinary research, and further developing mentor and expert networks. These plans aim to inspire continued engagement and innovation in environmental education.

The experience of scaling Ecoview from a national to an international initiative demonstrates its potential as a replicable model for integrating Earth observation into school-level science education while addressing complex global environmental challenges.

How to cite: Babiichuk, S., Dovgyi, S., and Davybida, L.: Expanding remote sensing–based environmental education: the Ecoview competition from national to international level, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2340, https://doi.org/10.5194/egusphere-egu26-2340, 2026.

The water–energy–food–ecosystems (WEFE) nexus is increasingly recognized as a promising approach to addressing ‘wicked problems’, that is, complex challenges marked by uncertainty and conflicting interests. Climate extremes are exposing vulnerabilities and trade-offs within the nexus, underscoring the need for co-designed, participatory governance approaches that move beyond sectoral silos and expert-driven decision-making. This approach emphasises social learning, knowledge co-production, and exchange as means of integrating scientific expertise, policy priorities, and local community perspectives. By fostering cross-sector collaboration, co-designed processes can generate trusted and actionable solutions that are responsive to both local and systemic challenges.

This study introduces a collaborative, multi-stakeholder framework to explore the vision of the WEFE nexus, identify key internal and external drivers of change, and co-design solutions and policy scenarios that reinforce interlinkages between nexus dimensions under climate change. Lake Como, northern Italy, serves as a case study due to competing water demands and increasing impacts of extreme weather events. Between October 2023 and February 2025, we conducted a series of dialogues with 20 key stakeholders representing each nexus dimension (e.g., lake operator, regional government, energy companies, irrigation districts, environmental platforms, municipalities). These dialogues combined semi-structured interviews, questionnaires, and workshops. Content analysis and statistical methods were used to examine stakeholders’ narratives, providing insights on 1) a shared vision of the nexus dimensions, 2) assessment of two policy scenarios: hydropower maximization and risk management, 3) evaluation of proposed solutions in terms of priority, relevance, effects on nexus dimensions, facilitation instruments, and implementation barriers, and 4) governance standards in the decision-making process.

The main findings show that nexus dialogues are a central vehicle for operationalising the WEFE nexus. They enabled a deeper understanding of the local context and associated needs, grounded nexus assessments in real-world conditions, and fostered social learning through stakeholders’ engagement. Stakeholders agreed that the nexus is fragile, highlighting the need to reinforce the green energy transition, innovate in food security, and better align human pressures across sectors. The two policy scenarios were analysed with respect to the benefits and impacts of each nexus dimension. Selected solutions –such as changes in hydropower licenses, adjustments in ecological flow standards, adaptations in lake management protocols, and insurance programs to address weather extremes– were evaluated based on stakeholders’ preferences. Governance analysis revealed the multifunctional roles of specific stakeholders (e.g., lake operator, irrigation districts, environmental associations), gaps in representativeness (e.g., mountain communities, municipalities), and participants’ aims to both negotiate and influence decisions. By placing stakeholder engagement at the core of co-designed policy scenarios, this work contributes actionable knowledge for policymakers and practitioners tackling WEFE nexus challenges in climate-exposed regions worldwide.

How to cite: Ricart, S. and Castelletti, A.: Co-Designed, Stakeholder-Driven Governance for the WEFE Nexus under Climate Extremes: Lessons from Lake Como, Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2541, https://doi.org/10.5194/egusphere-egu26-2541, 2026.

EGU26-3476 | Posters on site | EOS1.1

The Rocca di Papa (Italy) INGV Geoscience Museum: the last four years of activities  

Laura Colini, Valeria Misiti, Tommaso Alberti, Giuseppe Falcone, Tiziana Lanza, Antonella Megna, Antonella Cirella, Nicola Pagliuca, Luca Tarchini, and Massimo Ranaldi

The Geoscience Museum of Rocca di Papa (MuGeos), Italy, promotes science communication and education on behalf of Istituto Nazionale di Geofisica e Vulcanologia (INGV). The Museum is located at the centre of Alban Hills volcanic district, a dormant volcano whose last eruptive activity, an hydromagmatic phase, is dated about 20 ky ago. During the last four years the MuGeos has carried out activities dedicated to generic non expert public also joined with the municipality of Rocca di Papa, and to schools from Primary to Secondary.  All these activities belong to the so called Third Mission of INGV that consists of the diffusion of scientific knowledge. The education activity has been focused on the involvement of a significant number of schools coming from the surrounding territory but also from distant regions. The activity with students has consisted of an interactive and attractive guided tour through the knowledge of the Earth system (i.e. space weather, geomagnetism, seismology and volcanology, climate change), the Alban Hills Volcano, its origin hazard and peculiarities.  Moreover, the Museum has been involved in the Science Together Net project cofunded by the European Union through the organization of the European Researcher Night. In this context we have proposed activities involving kids, children and adults such as geotrekking on Alban hill volcano, seminars, labs of explosive and effusive volcanoes, paper volcanoes (origami) and fairy tales on geological myths, guided tours of the Museum, stars and planets observation through a telescope. The above mentioned activities have been proposed also during the Museum opening of every second Sunday of the month.  Further several activities dedicated to generic public have been promoted together with Rocca di Papa municipality in occasion of local events such as the October Chestnut Festival, the World Moon Day, the World Horse Festival, the Marconian Day Recurrence etc. During these popular events the MuGeos has been a fundamental actor in the awareness of citizens towards natural hazard and risks related to the territory.  Feedbacks of all the MuGeos activities are extremely positive; same teachers keep coming to the Museum every scholastic year, many positive public review on Google platform, satisfaction questionnaire.

How to cite: Colini, L., Misiti, V., Alberti, T., Falcone, G., Lanza, T., Megna, A., Cirella, A., Pagliuca, N., Tarchini, L., and Ranaldi, M.: The Rocca di Papa (Italy) INGV Geoscience Museum: the last four years of activities , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3476, https://doi.org/10.5194/egusphere-egu26-3476, 2026.

YouTube hosts several collections of videos that focus on topical geological topics. This presentation is concerned with viewer engagement around content on one of these. The Shear Zone channel, as of January 2026, has over 15k subscribers with over 1.25M views across its ~300 videos. Launched as a platform for sharing educational content aimed at university earth science students, over its five-year existence, films have evolved to a more documentary style and accessed increasingly by broader communities outside formal education environments. Although viewing figures, compared with some other popular YouTubers are not astronomical, some have attracted >>25k views with full views running at >18% (which is high for YouTube!). Comments are permitted, though moderated – which, along with “likes” and channel analytics – give insight on the reach, popularity, opinions and background of viewers.

To lever YouTube algorithms, content is monetised by permitting advertising at the start of each video but not with commercial breaks mid-programme, which can degrade viewer experience. Non-monetised content is marginalised by the platform. YouTube also has very strong recency bias in the content it reveals and it promotes content that attracts viewer engagement and retention. While there is long-term, recurrent viewer engagement for short-course teaching materials on The Shear Zone, views of the broader documentary style material generally die off after a few days. Very few users explore content by access channel home-pages or playlists – hence the preponderance of rather sensationalist thumbnails used by other content-creators to attract views. This presentation reports viewer engagement on a subset of content published on The Shear Zone channel.

In April-May 2024, the BBC’s broadcast the fourth series of Race Across The World, advertised as a journey through “The Ring of Fire in east and south-east Asia.  Independent of this, as the series developed, I dropped two videos each week, appropriate to that particular segment of the race, on YouTube. Meta-tagged to RATW, these covered topics as diverse as megathrust earthquakes and tsunamis, Holocene sea-level change, palaeogeographic assembly of SE Asia, volcanic eruptions and biogeography. Views ranged from around 2k to 25k, the most popular being a video on Krakatoa. Interestingly the tie-in to RATW seems to have yielded rather few views – most of the audience came from E and SE Asia!

More popular videos have attracted disproportionate comment from what politely might be called adherents to non-mainstream geoscience ideas – even when these are only tangentially associated with the video contents. Two films have attracted particular attention: The disappearing glaciers of Mont Blanc (published August 2022); and Trashing continental drift (in two parts; published September 2025). These commentaries provide useful insights on the types of evidence and information used by these communities and the challenge of communicating science when contested.

 

 

How to cite: Butler, R.: The Shear Zone Channel – reflections on sharing geological science on YouTube, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3525, https://doi.org/10.5194/egusphere-egu26-3525, 2026.

EGU26-3534 | Orals | EOS1.1 | Angela Croome Award Lecture

Sleepy cat and the cosmic dust: Lessons for non-fiction writing from 10 years as a magazine editor  

Joshua Howgego

To oversimplify things slightly, there are two types of story in journalism: the short ones and the long ones. I’ve spent much of my career so far focussed on the latter, known as features, which has meant an awful lot of head-scratching about how to keep readers engaged, excited, gripped by a story that goes on for several thousand words – no simple matter in the age of AI slop and TikTok.  

In this lecture, I’ll spill the beans on how we do things at New Scientist magazine, where I have worked for just over 10 years, with special reference to an idea known as “sleepy cat” from the mind of my brilliant former colleague Graham Lawton. I’ll also show how I used some of the tricks of creating compelling narratives in one of the stories in my book, The Meteorite Hunters – namely the tale of Jon Larsen, the Norwegian jazz guitarist who hunts cosmic dust on urban rooftops. 

Whether you want to better understand how journalists think, yearn to improve your own writing, or just enjoy thinking about how stories work, there should be something of interest here for you.

How to cite: Howgego, J.: Sleepy cat and the cosmic dust: Lessons for non-fiction writing from 10 years as a magazine editor , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3534, https://doi.org/10.5194/egusphere-egu26-3534, 2026.

EGU26-4107 | Orals | EOS1.1

Relaunching the Skeptical Science website to include prebunking tools 

Bärbel Winkler and John Cook

Skeptical Science is a highly-visited website featuring 250 rebuttals of misinformation about climate change and climate solutions. Many of the rebuttals are written at multiple levels—basic, intermediate, and advanced—in order to reach as wide an audience as possible. Results from a survey we've been running on our website since November 2021 indicate that there is some room for improvements in order to make the rebuttals more robust. It is therefore rather good timing that we've been working on a complete overhaul of our website which should increase the effectiveness of rebuttals in reducing acceptance in climate myths and increasing acceptance of climate facts. A key goal of misinformation interventions is to increase reader discernment, the difference between belief in facts and belief in myths. While there was overall an increase in discernment, with the decrease in agreement with myths greater than the decrease in agreement with facts, the result that belief in climate facts decreased for at least some rebuttals is unwelcome and counter to the goal of Skeptical Science. In this presentation, we'll give a sneak peek at how the new website will look like. One important new feature will be the inclusion - where applicable - of the fallacies employed by a climate myth, so that a rebuttal on the new website will then include all three elements of a successful debunking: fact, myth and fallacy. In my presentation, I'll also highlight some of the other updated or new features this website relaunch will include.

How to cite: Winkler, B. and Cook, J.: Relaunching the Skeptical Science website to include prebunking tools, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4107, https://doi.org/10.5194/egusphere-egu26-4107, 2026.

EGU26-5228 | Posters on site | EOS1.1

Keeping users in the loop: Outreach activities for ECMWF IFS and AIFS forecast model updates 

Milana Vuckovic, Becky Hemingway, Martin Suttie, and Victoria Bennett

ECMWF develops and maintains operational forecasting systems, which include the physics-based Integrated Forecasting System (IFS) and the Artificial Intelligence Forecasting Systems (AIFS Single and AIFS Ensemble). These models are upgraded periodically, delivering significant scientific and technical improvements, however these changes pose challenges for users who need to understand the implications to their workflows and applications and make required modifications.

Outreach activities combine structured documentation, targeted email notifications of key upgrade milestones, and LinkedIn and the ECMWF forum posts to reach wider audiences and gather feedback. These channels are complemented by series of webinars and presentations at the annual Using ECMWF's Forecasts (UEF) meeting, where technical and scientific upgrades are presented and discussed with users.

This presentation will describe ECMWF’s outreach activities around IFS and AIFS model upgrades, which are designed to support a diverse user community, including researchers, operational forecasters and developers of AI driven applications, among others. Lessons learned and key challenges will be presented, these include addressing the needs and expectations of diverse audiences with different levels of expertise, synchronising communication with operational timelines and maintaining consistent narratives across platforms, ensuring that key information is accessible without overwhelming users.

How to cite: Vuckovic, M., Hemingway, B., Suttie, M., and Bennett, V.: Keeping users in the loop: Outreach activities for ECMWF IFS and AIFS forecast model updates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5228, https://doi.org/10.5194/egusphere-egu26-5228, 2026.

EGU26-5425 | Posters on site | EOS1.1

User outreach and engagement at ECMWF: Examples of partnerships, outreach and innovation support 

Becky Hemingway, Milana Vuckovic, Cristina Ananasso, Chris Stewart, Julia Ioannu, Athina Trakas, Olga Loegl, and Stijn Vermoote

ECMWF’s Partnerships and Engagement section supports the effective use of ECMWF, Copernicus and Destination Earth services, datasets and infrastructure through partnerships and many targeted outreach and engagement activities. This work serves a diverse user community, including the National Meteorological Services (NMS) of ECMWF Member and Co-operating States (MS and CS), EU Member States, EU institutions and agencies, and WMO and other UN bodies, as well as a growing community of researchers, private companies, weather enthusiasts and other users.

This poster presents selected examples of outreach and engagement activities and shows how different approaches are combined to respond to evolving user needs and to build sustained dialogue with user communities. Liaison visits to ECMWF MS and CS NMSs support long-term collaboration and enable direct discussions on ECMWF activities including operational needs of forecasters. Further engagement is delivered through the Copernicus CAMS and C3S National Collaboration Programmes, which aim to strengthen the links with National Partner institutions and increase the uptake of Copernicus services at country level. In addition, the first two Copernicus Thematic Hub pilots, which focus on health and energy, are demonstrating the value of targeted outreach and support across these sectors.

Training activities are a key part of ECMWF's outreach and cover topics ranging from Numerical Weather Prediction and machine learning to software development and high-performance computing. Experience shows that combining clear explanations with practical examples is important for supporting users with different backgrounds and levels of experience, especially in an increasingly open science environment.

ECMWF Outreach also includes activities around ECMWF’s forecast model upgrades, such as updates to the Integrated Forecasting System (IFS) and the Artificial Intelligence Forecasting System (AIFS) in the medium, sub-seasonal and seasonal forecast ranges. These activities focus on communicating and explaining scientific and technical developments in the models and how they may effect user workflows, new forecast products, and how the updated models perform based on evaluation results.

Code for Earth programme offers hands-on, challenge-based opportunities for participants to develop innovative applications using ECMWF, Copernicus and Destination Earth data and software. The AI Weather Quest is a real-time international competition in which participants submit AI-based sub-seasonal forecasts in an operational-like setting, with results evaluated through transparent and openly documented methods.

How to cite: Hemingway, B., Vuckovic, M., Ananasso, C., Stewart, C., Ioannu, J., Trakas, A., Loegl, O., and Vermoote, S.: User outreach and engagement at ECMWF: Examples of partnerships, outreach and innovation support, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5425, https://doi.org/10.5194/egusphere-egu26-5425, 2026.

EGU26-5542 | ECS | Posters on site | EOS1.1

Graphic novel communicates changes in Arctic landscapes, fostering wonder and curiosity 

Domino Jones, Nina Kirchner, and Johanna Dahlkvist

The Arctic has long captured the imagination through its remoteness, wildlife, striking landscapes, and rich cultural histories. At the same time, Arctic environments are undergoing rapid and profound changes, with many landscapes expected to be transformed beyond contemporary recognition by the end of this century. Communicating these changes to non-specialist audiences presents a significant challenge: they unfold across vast spatial and temporal scales, are studied through multiple disciplinary lenses, and resist simple or singular narratives. From ancient glaciers to pioneering lichen, no single process exists in isolation. Rather, Arctic change emerges through the interaction of glaciological, geological, botanical, fluvial, and meteorological processes. Understanding and communicating this complexity requires approaches that can hold multiple perspectives together while making these remote landscapes emotionally accessible and relevant to the audience.

We present ‘Arctic Flowers’, a science communication graphic novel which explores changing Arctic landscapes through the lived experiences of scientists working in the Tarfala Valley of northern Sweden. As most of Sweden’s glaciers face complete disappearance before the year 2100, this story captures a pivotal moment in the region’s history. Rather than adopting a purely catastrophic narrative, ‘Arctic Flowers’ foregrounds nuance, emotional connection, and scientific practice through non-fiction visual storytelling. The narrative follows researchers at Tarfala Research Station as they document retreating glaciers and the parallel emergence of Arctic flora. A central narrative thread connects contemporary research to a rediscovered herbarium created in the 1960s by botanist Adélaïde Stork, allowing readers to grasp climate change through intergenerational scientific observation and long-term data.

Graphic novels offer a powerful medium for science communication, particularly for topics that span multiple spatial and temporal scales. Through the juxtaposition of panels, text, and imagery, multiple concepts can be laid out on the page together, encouraging reflection and synthesis from the audience. Shifts in perspective, scale, and framing are used to emphasize grandeur at multiple scales, from larger-than-life structures such as mountains, glaciers, and research station operations to small, attentive details—the textures of plants and rocks, or the correct way to hold an ice axe. By blending scientific data, historical context, personal experience, and observation of the landscape, the project aims to spark curiosity and invite readers to ask questions about the changing Arctic. This mirrors the inquisitive and exploratory approach practiced by scientists within the story, drawing on first-hand accounts and interviews with generations of researchers at Tarfala Research Station – their experience spanning six decades. We reflect on lessons learned from developing this work as a long-form science communication effort, including how narrative and character-driven inquiry can foster emotional engagement, encourage dialogue, and make Earth science accessible and meaningful to diverse audiences.

How to cite: Jones, D., Kirchner, N., and Dahlkvist, J.: Graphic novel communicates changes in Arctic landscapes, fostering wonder and curiosity, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5542, https://doi.org/10.5194/egusphere-egu26-5542, 2026.

EGU26-6304 | Posters on site | EOS1.1

Slow Science Communication 

Siska Van Parys, Stijn Pardon, and Reinout Verbeke

Most science communication today is short and fast — but at the Institute of Natural Sciences we also try something different. Together with colleagues, Siska Van Parys works on long-form stories that highlight the institute’s core research areas — palaeontology, geology, archaeology, taxonomy, evolution — and the collections that support them. They create overview articles on the website, mini-documentaries about expeditions and fieldwork, and stories that put the spotlight on the people behind the research. 

Siska will share some of the projects she’s been involved in, what they hope to achieve with them, and why slow science communication has become part of the approach of the Institute of Natural Sciences.

The main examples will revolve around two geology projects: ROBOMINERS and LEAP. These scientific projects, carried out by the geologists of the Institute of Natural Sciences (Giorgia Stasi, Christian Burlet, Sophie Verheyden), were followed and documented by Siska and her colleagues. The results are two mini-documentaries and long-reads. 

How to cite: Van Parys, S., Pardon, S., and Verbeke, R.: Slow Science Communication, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6304, https://doi.org/10.5194/egusphere-egu26-6304, 2026.

Over the past decade, we have carried out sustained outreach activity on social media aimed at presenting seismic data to students and the general public. The primary goal has been not only to increase the visibility of Earth sciences, but also to highlight the fundamental role of data acquisition in subsequent scientific tasks, such as numerical modeling and tectonic interpretation. A significant part of this effort has focused on visualizing seismic waves generated by local, regional, and teleseismic earthquakes, often using data recorded by the GEO3BCN Educational Seismic Network deployed in northeastern Spain. These activities are particularly valuable in regions characterized by low to moderate seismicity, where public familiarity with earthquakes is generally limited.

Beyond earthquake-related content, we have also shared posts illustrating ground vibrations generated by non-tectonic natural processes and anthropogenic sources. Topics related to environmental seismology often attract strong public interest, as it is not widely known that natural phenomena such as tides, ocean waves, rainfall, wind, and thunder can be monitored using seismic data. Similarly, vibrations induced by human activity -from student movement between classrooms to crowd dynamics during music concerts or football matches- tend to generate considerable attention, sometimes even reaching mass media coverage. We leverage this curiosity as an opportunity to bring seismology, and Earth sciences more broadly, closer to society.

This work has benefited from partial support of the EPYSIM Project, funded by the Spanish Ministry of Science and Innovation (Ref.: PID2022-136981NB-I00).

How to cite: Diaz, J.: A long-term review of outreach activity on social media related to seismic data , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6484, https://doi.org/10.5194/egusphere-egu26-6484, 2026.

EGU26-7163 | ECS | Posters on site | EOS1.1

Altra Quota: a field-based monitoring and education initiative for Disaster Risk Management in the Western Italian Alps 

Vittorio Giordano, Maria Elena Alfano, Luigi Cafiero, Nike Chiesa Turiano, Martina Leone, Flavia Marini, and Andrea Vito Vacca

Effective Disaster Risk Management (DRM) education requires geoscientific knowledge to be grounded in local contexts and translated into practical skills for those involved in risk prevention and emergency response. Altra Quota is a monitoring initiative in the Western Italian Alps that integrates real-time environmental monitoring, field-based research, and dissemination activities. It operates through close collaboration with local administrations and stakeholders exposed to hydro-meteorological, hydrogeological and cryospheric hazards.

A core aim of the project is to support capacity building in DRM through risk communication and the dissemination of monitoring results. Data from hydrological, meteorological and geomorphological monitoring networks are actively employed in hands-on activities for students, practitioners and decision-makers, enabling participants to interpret real-world observations, understand early warning systems and explore decision-making under uncertainty. Through field-based training, laboratory activities and dissemination initiatives, the project bridges theoretical geoscientific concepts with operational DRM practices. These activities empower local communities to better understand risks and interpret information from monitoring and warning systems, which is crucial for effective prevention and rapid response to emergencies.

A key component of the project is the long-term monitoring of the Ciardoney Glacier, conducted in collaboration with the Italian Meteorological Society. The glacier’s retreat and the resulting hydrological stress offer a powerful case study to analyze and communicate the impacts of climate change on alpine water resources and downstream risks. By combining observations from ground stations, satellite data, and model simulations, the researchers from Altra Quota can offer engaging experiences that effectively contextualize hazards.

Ultimately, by linking scientific research, education, and community engagement, Altra Quota represents a model for DRM education that improves risk awareness, strengthens the dialogue between science and society, and supports informed decision-making under changing climatic conditions.

How to cite: Giordano, V., Alfano, M. E., Cafiero, L., Chiesa Turiano, N., Leone, M., Marini, F., and Vacca, A. V.: Altra Quota: a field-based monitoring and education initiative for Disaster Risk Management in the Western Italian Alps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7163, https://doi.org/10.5194/egusphere-egu26-7163, 2026.

Belgium's compact territory contains an exceptionally rich geological record. Through repeated collisions and tectonic upheavals during our long journey from the southern hemisphere, layers from nearly every period of the past half billion years are exposed at the surface. The Planet Belgium project explores this remarkable geological heritage through a multimedia approach combining five immersive podcast episodes, five longread articles in popular science media, and five educational posters. Longreads are in Dutch, French and English.

In each episode and article, we venture into the field with Belgian experts and citizen scientists. Step by step, we reconstruct the sequential building of Belgium's subsurface through deep time. The project aims to convey a sense of wonder about geology and encourage audiences to see "boring" stones with new eyes.

Featured geological elements include Belgian whetstones and cobblestones, the famous red and black Belgian marble, bluestone, coal - our former "black gold" - and chalk, among others. The spectacular fossil collections at the Royal Belgian Institute of Natural Sciences in Brussels, including the world-famous Bernissart Iguanodons, tell the evolutionary history of life on Earth from the Cambrian up until the last Ice Age, bringing these ancient worlds to life for modern audiences.

This presentation (oral or in a poster session) will discuss the strategies employed to make deep time accessible and engaging across multiple formats (podcast, ‘scrollitelling’, posters, teaser videos), the challenges of translating expert knowledge for public audiences, and the role of aesthetic design in science communication. I will share lessons learned and evaluate the project's success.

The first episode is published here: https://www.naturalsciences.be/r/planetbelgium
Three episodes will be online at the time of the conference. 

How to cite: Verbeke, R. and Piessens, K.: Planet Belgium: narrating the geological odyssey of a country through multimedia storytelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7191, https://doi.org/10.5194/egusphere-egu26-7191, 2026.

The energy transition from fossil fuels to low-carbon energy systems is a crucial global aspect requiring sustainable and urgent solutions directed toward the use of renewable resources, such as geothermal energy. The general public still has little knowledge of geothermal energy, despite its advantages: misconceptions about safety, environmental impacts, and technological feasibility continue to hinder its wider adoption. To overcome these challenges, timely, transparent, and easily accessible public engagement strategies are required. In this scenario, translating complex geoscientific phenomena into stories that the general public can understand is key and demands effective science communication. An efficient way to promote interest and understanding is to combine scientific content with visual storytelling and illustration.
This poster outlines the creation of “The Magical Heat of the Earth”, an illustrated book for primary school students designed to convey the concept of geothermal energy and its application as an energy resource. The book was authored, designed, and illustrated at INGV (Istituto Nazionale di Geofisica e Vulcanologia, Italy) through ongoing collaboration between the geoscientist and the designer/illustrator. This analysis emphasises the creative and methodological processes involved in the product’s creation rather than focusing on the final outcome alone. The creative process is described as progressing from the initial scientific concept and narrative framework to visual research, character design, storyboard development, and final layout design, illustration, and typesetting. Significant focus is placed on the interaction between the scientist and the designer/illustrator, and on the balance achieved between scientific and artistic precision throughout the process. The case study indicates that using handcrafted, research-based illustrations remains an effective method for conveying scientific concepts, particularly to children. The authors reflect on simplification, the use of rhyming texts and visual metaphors, and emotional engagement as significant methods for educating individuals about science, particularly in fostering interest in geothermal energy and Earth sciences overall.

How to cite: Florindo, F. and Procesi, M.: From Geoscience to Visual Storytelling: an Illustrated Children’s Book to Communicate Geothermal Energy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7204, https://doi.org/10.5194/egusphere-egu26-7204, 2026.

EGU26-7398 | Posters on site | EOS1.1

Visualizing Science: The Role of Graphic Design in Educational and Outreach Activities at INGV 

Giuliana D'Addezio, Daniela Riposati, Francesca Di Laura, Patrizia Battelli, Federico Florindo, and Gianluca Nardi

One of the core missions of the Istituto Nazionale di Geofisica e Vulcanologia (INGV) is to promote awareness of geophysics and natural hazards through education and outreach. Central to this mission is the Laboratorio Grafica e Immagini, INGV’s primary hub for visual communication. Over the past five years, the laboratory has taken on an increasingly strategic role in bridging the gap between scientific research and public understanding.

This work presents a selection of educational materials—including books, scientific games, infographics, illustrated brochures, and interactive exhibits—designed to explain seismic, volcanic, and environmental phenomena to diverse audiences, ranging from school groups to the general public. Each product is developed in close collaboration with scientists to ensure accuracy, while leveraging visual storytelling techniques to enhance clarity and engagement.

Our work demonstrates that graphic design is not merely a supporting function, but a vital component of scientific communication—particularly in educational contexts, where visual language significantly improves learning and retention. We also reflect on key challenges, such as simplifying content without compromising accuracy, and designing for inclusivity. This contribution underscores the value of interdisciplinary collaboration between scientists and designers in achieving effective and impactful outreach.

How to cite: D'Addezio, G., Riposati, D., Di Laura, F., Battelli, P., Florindo, F., and Nardi, G.: Visualizing Science: The Role of Graphic Design in Educational and Outreach Activities at INGV, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7398, https://doi.org/10.5194/egusphere-egu26-7398, 2026.

EGU26-7827 | ECS | Orals | EOS1.1

Using sequential art to communicate scientific ocean drilling 

C. Nur Schuba, Sara Satolli, Natsumi Nakano, Morgane Brunet, Piero Bellanova, and Maria Jose Jurado and the Expedition 405 and 502E Scientists

Scientific ocean drilling offers a unique window into Earth processes that cannot be accessed through surface observations alone, but its remote offshore setting and technical complexity pose challenges for public communication. International drilling programs such as the International Ocean Discovery Program (IODP) and the International Ocean Drilling Programme (IODP3) are also inherently multinational and multilingual, yet these collaborative dimensions are not always reflected in expedition outreach materials.

This presentation introduces Chikyu Chronicles, a two-volume comics-based outreach project developed for IODP Expeditions 405 and 502E in the Japan Trench. The project uses illustrated sequential narratives to communicate shipboard science, engineering workflows, and everyday expedition life to middle-grade audiences while remaining grounded in real people, roles, and practices. Rather than emphasizing scientific results, the comics focus on portraying scientific ocean drilling as a collaborative activity shaped by operational constraints and teamwork. Each volume combines comics with book back matter designed to extend engagement beyond the narrative. Photographic sections document shipboard spaces, tools, and activities, allowing readers to connect simplified illustrations they have encountered in the book to physical environments and scale. Activity-based back matter invites participation through creative and interpretive exercises, including making science comics and identifying plate boundary patterns using multiple geophysical and geological datasets. Together, these elements form a hybrid communication model that supports place-making and causal reasoning.

Production of Chikyu Chronicles was embedded within the expedition environment and extended after sailing through distributed collaboration. Expedition participants contributed through interviews, reference materials, scientific review, editorial feedback, and translation assistance, ensuring linguistic accuracy and contextual fidelity without separating communication from scientific practice. Reported outcomes so far are qualitative and formative, drawing on informal feedback and basic reach metrics from real-time dissemination during Expedition 405, with structured audience evaluation currently underway. The project illustrates how comics-based outreach can align communication practices with the collaborative realities of international geoscience research.

How to cite: Schuba, C. N., Satolli, S., Nakano, N., Brunet, M., Bellanova, P., and Jurado, M. J. and the Expedition 405 and 502E Scientists: Using sequential art to communicate scientific ocean drilling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7827, https://doi.org/10.5194/egusphere-egu26-7827, 2026.

EGU26-7980 | Posters on site | EOS1.1

The 2024 Collectors Tour: A Case Study in Field-Based Geoscience Communication 

Jeffrey Munroe and Andrew Cassel

The “2024 Collectors Tour” was a field-based science communication initiative that employed narrative structure, place-based explanation, and methodological transparency to bring Critical Zone science alive for a non-specialist audience.  The Collectors Tour consists of a 21-episode video series produced during an 18-day, 4,500-km field campaign to empty mineral dust collectors deployed across Utah, Nevada, and Idaho in the southwestern United States.  This work was part of the DUST^2 project, funded by the US National Science Foundation to investigate the role of mineral dust erosion, transport, and deposition in the geoecological functioning of Earth surface environments (i.e. the “Critical Zone).  Each video of the Collectors Tour was anchored to the location where a specific dust collector is deployed, and used that location to introduce concepts related to mineral dust, soil formation, snow hydrology, climate variability, ecosystem function, and human influence.  In this way, the Collectors Tour embedded scientific explanation directly within active fieldwork, inviting viewers to observe how geoscience knowledge is generated in real settings.  The strategy of multiple sequential videos, produced and distributed in rapid succession, emphasized authenticity, continuity across episodes, and visual engagement with landscapes, transforming the routine annual campaign to service the dust collectors into a coherent outreach narrative.  The Collectors Tour also reflected lessons learned from long-term communication efforts, including the value of consistency, the power of storytelling grounded in genuine field practice, and the importance of acknowledging collaboration, logistics, and uncertainty.  To date the videos have received more than 2600 total views, making this a broadly successful and lasting science outreach success.​  As a case study, the Collectors Tour offers a replicable model for integrating science communication into ongoing field research and contributes to broader discussions on effective strategies for communicating science to diverse audiences. 

How to cite: Munroe, J. and Cassel, A.: The 2024 Collectors Tour: A Case Study in Field-Based Geoscience Communication, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7980, https://doi.org/10.5194/egusphere-egu26-7980, 2026.

Pollution of English waterways by untreated sewage discharged through Combined Sewer Overflows (CSOs) has become one of the most high-profile environmental issues in the UK. It is now a major political topic, featuring prominently in election campaigns, parliamentary inquiries, and resulting in new legislation. To better communicate this environmental issue and empower the public to take action against it, we created www.SewageMap.co.uk a user-friendly, real-time visualisation of sewage spills across England. SewageMap uniquely combines live CSO data with a hydrological model to identify rivers downstream of recent spills, making it particularly valuable for recreational water users such as swimmers, kayakers, and rowers. The platform is recommended by organisations representing these groups and is widely used by citizen scientists and campaigners.

To make the experience engaging and relatable, SewageMap makes prodigious use of playful design elements, including the ‘poop’ and other emojis to highlight the ‘gross’ nature of sewage pollution. Behind the scenes, SewageMap is powered by 'POOPy' (Pollution Discharge Monitoring in Object-Oriented Python), an open-source toolkit that standardises diverse CSO datasets and enables historical spill analysis. Data generated by POOPy has supported river protection groups and informed local planning meetings; we believe that data from SewageMap has even featured in parliamentary debates.

The website was developed with both desktop and mobile users in mind, validated by the fact that ~80% of users access SewageMap via mobile or tablet devices. This ensures accessibility for the majority of users and highlights that this should be a consideration for other web visualisations. Furthermore, SewageMap can be embedded within external pages, which has enabled major news organisations to integrate the map into articles, significantly amplifying its reach.

The impact of this tool has been substantial, and greater than expected when the project was started informally. The site has received over 300,000 visitors in the past 12 months, financial support from major NGOs such as RiverAction, and resulted in new collaborations across academic and non-academic sectors. Overall, these projects have emphasised, to us, how engaging design, accessibility & proactive engagement with a user-base can result in significant impact stemming from a relatively ‘simple’ scientific principle.

How to cite: Lipp, A. and Dawe, J.: www.SewageMap.co.uk and POOPy: Open-source tools for understanding and communicating the impacts of sewage pollution on waterways in real-time, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7995, https://doi.org/10.5194/egusphere-egu26-7995, 2026.

EGU26-8024 | Orals | EOS1.1

“Signals from the climate in FVG”: a magazine enhancing climate awareness and bridging the gap between science and society at the regional level 

Federica Flapp, Fulvio Stel, Elena Caprotti, Nicolò Tudorov, Silvia Stefanelli, Giovanni Bacaro, Renato R. Colucci, Lorenzo Consorti, Filippo Giorgi, Alessandro Peressotti, Fabio Raicich, and Cosimo Solidoro

The informative publication “Segnali dal Clima in FVG” (Signals from the climate in FVG) provides a local and regional perspective on climate change, specifically tailored for the citizens of Friuli Venezia Giulia region (northeastern Italy). Structured around three core themes - Changes, Impacts and Actions - the publication serves as a bridge between the scientific community and the general public.

VISION AND COLLABORATION

This initiative stems from the Clima FVG Working Group*, a collaborative network of the region’s leading scientific and research institutions. The group operates on the principle that technological and scientific progress must be accompanied by public awareness and education to effectively tackle climate challenges. By translating complex data and information into an engaging, accessible format, the publication bridges the gap between expert research and citizen understanding.

CONTENT AND EDITORIAL APPROACH

Designed as an annual popular science magazine, the publication explores a wide array of climate-related themes, including the cryosphere, marine and lagoon ecosystems, forestry, wildlife and terrestrial ecosystems, agriculture, human health and urban settlements, as well as the psychological and social dimensions of climate change. Each issue explores a diverse range of topics, while remaining anchored to some core principles and maintaining key defining features:

  • Local-to-Global Connection: by recalling recent local weather events and by linking regional climate trends to the global climate change, the publication makes a far-reaching issue feel immediate and relevant to the local community;
  • Accessible Storytelling: by providing mini-glossaries, clear explanations, infographics and practical examples, the editorial project enables non-expert readers to understand complex topics without oversimplifying them;
  • Empowerment over Anxiety: by highlighting actionable mitigation and adaptation strategies at both individual and collective levels, the magazine frames climate issues through a constructive lens, aiming to reduce climate-related anxiety and to inspire climate action.

PRODUCTION AND STRATEGIC VALUE

Coordinated by ARPA FVG, the magazine is produced entirely "in-house" through the voluntary contributions of the experts, without dedicated external funding. While the publication is freely available online, limited print editions are produced for policymakers and institutional use.

Beyond its educational role, “Segnali dal Clima in FVG” serves as a vital networking tool. The collaborative drafting process fosters interdisciplinary relationships among experts and generates a localized knowledge base that is instrumental in shaping regional climate policy and resilience strategies.

AVAILABILITY

Segnali dal clima in FVG is available at https://www.arpa.fvg.it/temi/temi/meteo-e-clima/sezioni-principali/cambiamenti-climatici/segnali-dal-clima-in-fvg/

The complete PDF version can be browsed online or downloaded. Additionally, individual thematic sections from each edition and summary materials are available for download. The magazine is also being distributed to schools across Friuli Venezia Giulia through the regional environmental education network.

 

*THE CLIMA FVG WORKING GROUP

The Clima FVG Working Group brings together the premier scientific and research institutions working on climate change in Friuli Venezia Giulia region: the Universities of Trieste and Udine, CNR-ISMAR, CNR-ISP, ICTP, OGS. The group was formally established in 2022 by the Autonomous Region Friuli Venezia Giulia and is coordinated by the Regional Environmental Protection Agency – ARPA FVG.

How to cite: Flapp, F., Stel, F., Caprotti, E., Tudorov, N., Stefanelli, S., Bacaro, G., Colucci, R. R., Consorti, L., Giorgi, F., Peressotti, A., Raicich, F., and Solidoro, C.: “Signals from the climate in FVG”: a magazine enhancing climate awareness and bridging the gap between science and society at the regional level, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8024, https://doi.org/10.5194/egusphere-egu26-8024, 2026.

EGU26-8179 | ECS | Posters on site | EOS1.1

Beyond Data: Connecting People to Sustain the Relevance of Flux Science - Insights from the Meet the Fluxers podcast 

Laurent Bataille, Jessica L. Richardson, Maoya Bassiouni, Shannon A. Carnevale, Lara B. Milligan, Jessica Steier, Jarrod Breithaupt, Zingfa Wala, Qing A. Saville, Emma Reich, Robert Shortt, Tyler D. Roman, Maricar Aguilos, and Sung-Ching Lee

Eddy-covariance (EC) flux towers have collected decades of data on carbon, water, and energy exchanges, helping us understand how ecosystems respond to climate change. However, a gap persists between EC research outputs and how this knowledge reaches societal groups. The Meet the Fluxers podcast addresses this gap by connecting flux scientists with stakeholders and communities in shared ecosystems, making flux science accessible to the general public in a broader, more applied context.


While flux measurements are technically complex, and communication among relevant groups can be fragmented, many researchers are already overcoming these challenges through collaborative practice. The podcast gives voice to these researchers who are co-creating fluxscience with land managers, policymakers, and local communities, building trusted relationships that make science more relevant and actionable. By showing these real examples, the podcast educates listeners, clarifies limitations and demonstrates how collaborative engagement transforms both research and practice, particularly in under-monitored regions and rapidly changing ecosystems facing budgetary pressures.


To better understand the impact of science podcasts, Spotify analytics and transcript extraction were used to analyze audiences across four podcasts (Meet the Fluxers, Unbiased Science, Naturally Florida, and On the Trail of Science). The audiences primarily consist of millennials and are more frequently female, with listening geographies expanding beyond host locations. Engagement is non-linear, reflecting episodic releases. Transcript analysis shows listener interest is influenced by theme, place, narrative, and personal experience. These findings suggest that long-form audio formats can broaden access through repeated, place-based engagement. In addition to improved data products, relational communication formats are essential for maintaining relevance amid rapid environmental change and political uncertainty.

How to cite: Bataille, L., Richardson, J. L., Bassiouni, M., Carnevale, S. A., Milligan, L. B., Steier, J., Breithaupt, J., Wala, Z., Saville, Q. A., Reich, E., Shortt, R., Roman, T. D., Aguilos, M., and Lee, S.-C.: Beyond Data: Connecting People to Sustain the Relevance of Flux Science - Insights from the Meet the Fluxers podcast, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8179, https://doi.org/10.5194/egusphere-egu26-8179, 2026.

EGU26-8270 | Posters on site | EOS1.1

GeoHikes: Lessons from a long-term, place-based geoscience communication initiative in Ontario, Canada 

Alexander L. Peace, Daniel Dick, Carolyn Eyles, Elli Papangelakis, Katie Maloney, Deana Schwarz, Bernard Kradjian, Veronica Klassen, and Bill Pearson

GeoHikes is a place-based geoscience communication initiative designed to connect non-specialist audiences with geoscience through short outdoor experiences supported by accessible digital resources. Developed through partnerships between academics, professional geoscientists, educators, and community organisations, GeoHikes combine self-guided walks with mobile-friendly virtual field trips that highlight geoscience in familiar landscapes, including urban settings and recreational trails. These virtual field trips can be viewed on http://geoscienceinfo.com

Over the past decade, the programme has expanded to nearly 60 virtual field trips across Ontario, reaching diverse audiences through in-person engagement, online platforms, and public events. We reflect on the key challenges and successes of sustaining and scaling a long-term geoscience communication effort, including co-creation with communities, balancing scientific rigour with accessibility, and fostering emotional connection through place and narrative. We discuss lessons learned and identify transferable approaches for effective, community-centred geoscience communication.

How to cite: Peace, A. L., Dick, D., Eyles, C., Papangelakis, E., Maloney, K., Schwarz, D., Kradjian, B., Klassen, V., and Pearson, B.: GeoHikes: Lessons from a long-term, place-based geoscience communication initiative in Ontario, Canada, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8270, https://doi.org/10.5194/egusphere-egu26-8270, 2026.

Democracies face a dual challenge. On the one hand, democratic institutions are increasingly under pressure from authoritarian, right-wing populist, and extremist actors. On the other hand, socio-ecological transformation in response to climate change requires decisive action, social solidarity, and trust in democratic institutions. These processes are intertwined: ecological crises - particularly extreme weather events - may foster democratic resilience but can also intensify authoritarian backlash, thereby undermining transformation efforts. Given that the entire science enterprise has come under attack, the question is what role should or could academics play to fight the backlash and to resist the onslaught on intellectualism and facts?

As a follow-up from last year’s short course on academic activism, here I am presenting results of a perspective piece that is analysing the current political status quo in the US based on state-of-art of behavioural and social science research. We shed light on the academic response to Trumpism and how the authoritarian onslaught has affected climate science. We provide recommendations as to how one can deal with bad-faith actors and how one can identify them to begin with? How do we change our way to communicate and rise to the challenge? How do we regain ground, get organised and bring about the necessary discomfort? In order to understand the dynamics, we dissect critical factors such as emotions, biases, neurological and psychological disorders. We discuss social shifts from a current and historical perspective. We shed light on the role of the media (legacy as well as social media). And ultimately, we offer solutions for how to communicate more effective and goal-oriented. 
In a climate as well as societal context.

How to cite: Haustein, K.: Science communication and academic activism in times of rising authoritarianism and Trumpism., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8368, https://doi.org/10.5194/egusphere-egu26-8368, 2026.

EGU26-8373 | Orals | EOS1.1 | Katia and Maurice Krafft Award Lecture

What we’ve learned from teaching people in prison to Think Like a Scientist  

Philip Heron and the Think Like A Scientist team

Scientific thinking requires the critical analysis of information, while science itself thrives on the diversity of ideas. Yet, science, technology, engineering, and math (STEM) subjects have historically struggled to be inclusive and accessible to students from underrepresented communities - meaning we often miss a diversity of voices. Furthermore, STEM subjects have often been rigid in their teaching structure, creating barriers to education for students with more specific (or unrecognised) learning needs.

To address this, our science outreach course Think Like A Scientist was designed to improve critical thinking and encourage independent thought by applying adaptive education practices to create inclusive and accessible classroom environments. The program started in 2017 and has been applied in several different settings (e.g., schools and adult learning centres), but has mainly featured in prisons around the world (including England, Canada, Australia, and Spain).

Our students in prison often have a complex relationship with learning – such as low confidence in themselves or the education system (which is also a common trait amongst STEM university students from diverse communities). In addition, a classroom can present numerous other barriers for prison students (e.g., sensory, communication, information processing, and regulation) which particularly impacts neurodivergent learners (e.g., autism, ADHD, OCD, dyslexia, etc.). In our teaching in prison, we have been conscious of creating different educational access points that are not solely reliant on rigid teaching structures.

In this Katia and Maurice Krafft Award talk, I will outline the choices we have made in prison education to increase educational engagement - and how these choices can map onto other avenues of science communication to widen STEM participation. I’ll also share the impact of such practices on our students and how placing learners at the centre of education can be transformative.  

Fundamentally, as a society we need an informed population of any background who can think critically, especially in today’s world of fake news. In our sessions, we replicate this through learning from each other to Think Like A Scientist.

How to cite: Heron, P. and the Think Like A Scientist team: What we’ve learned from teaching people in prison to Think Like a Scientist , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8373, https://doi.org/10.5194/egusphere-egu26-8373, 2026.

EGU26-9110 | Posters on site | EOS1.1

Geoscience awareness in educational and outreach contexts: a preliminary analysis 

Linda Morgissi and Michele Lustrino

Communication and education in the geosciences are key elements for increasing awareness of natural hazards, fostering an integrated understanding of the Earth system, and improving natural resource management. Despite this, several studies highlight a persistent misalignment between the societal importance of geology and the way this discipline is commonly perceived by the public.

This study aims to explore how geological topics are received and interpreted by different audiences, representing an important step for the design of effective educational and outreach actions. The contribution presents preliminary results from a survey conducted within a broader PhD research project, focused on geoscience communication and outreach.

Two paper-based questionnaires, each consisting of 15 multiple-choice questions with four options and a single allowed answer, were developed and administered to a sample of approximately 220 children and 250 adults (including parents and teachers). Participants were involved in educational and outreach activities organized by the Department of Earth Sciences (DST) of Sapienza University of Rome. The survey was conducted in Rome and Central Italy. The adult questionnaire investigated themes related to geological awareness, Earth system processes, natural hazards, climate change, lifestyles, and the use of natural resources. The children’s questionnaire, stratified by school grade, focused on basic geological concepts, including rocks, fossils, minerals, volcanoes, and earthquakes.

Preliminary results, based on an ongoing dataset, are presented separately for the two target groups. Among adults, responses indicate a tendency to interpret geoscientific topics primarily through interpretative frames, related to natural hazard mitigation and sustainability. These perspectives appear to reflect widely shared societal narratives, rather than an integrated understanding of geological processes operating across different spatial and temporal scales. Children’s responses, while often grounded in intuitive or narrative reasoning, show an overall solid understanding of some key concepts, particularly when supported by direct and hands-on experiences. In both samples, understanding of geological topics appears heterogeneous, context-dependent, and influenced by school-based learning and media exposure.

These initial findings highlight the importance of developing educational and outreach strategies that take existing interpretative frames into account and promote integrated, experiential, and territorially contextualized activities. Data collection is ongoing and will be extended to additional contexts and methodological approaches, supporting the progressive refinement of outreach and educational actions within the PhD project.

 

 

How to cite: Morgissi, L. and Lustrino, M.: Geoscience awareness in educational and outreach contexts: a preliminary analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9110, https://doi.org/10.5194/egusphere-egu26-9110, 2026.

EGU26-9213 | Posters on site | EOS1.1

The Potsdam WaterHub - Research, Networking, Training and Outreach 

Jürgen Mey, Bodo Bookhagen, Jan Haerter, Georg Feulner, and Thorsten Wagener

Europe's climate is warming faster than any other region of the world. This accelerated  warming has severe consequences for water resources and water extremes. Heatwaves occur more frequently and intensively, and extreme events such  as droughts and heavy rainfall are increasing considerably. For Europe, we expect that an atmospheric temperature increase of 2°C would double economic losses from flooding while economic losses from droughts might  triple. Whereas regions in southern Europe and the Mediterranean already experience frequent droughts, wetter regions such as Germany will experience particularly dramatic changes in hydro-climatic conditions.

Within Germany, challenges for managing water during dry periods are particularly evident in the state of Brandenburg in Eastern Germany. Low annual precipitation and sandy soils with low water storage capacity characterize this region, which is considered both “water-rich and water-poor” for good reasons. Increasing impacts of anthropogenic climate change will likely lead to changing rainfall and evaporation patterns, with consequences for water supply to soils, rivers and groundwater aquifers. We can expect more stress for aquatic ecosystems due to changing river flows, while changing soil moisture and groundwater levels will negatively impact agriculture, forests and terrestrial ecosystems. Furthermore, in the coming decades, large areas of southern Brandenburg will have to compensate for a massive water deficit caused by decades of groundwater pumping in the context of lignite mining.

The Potsdam WaterHub was established as a cross-institutional platform to support and connect water researchers in Potsdam. Potsdam provides an ideal starting point for such an initiative, given its high density of internationally recognized research institutions and long-standing expertise across the water sciences. We will present our strategy to foster interdisciplinary exchange, collaborative research, involvement in BSc/MSc training and innovation to advance understanding of complex water systems and risks. In addition, the WaterHub actively engages with the public, media, policy-makers, and stakeholders from industry and practice, contributing scientific knowledge and dialogue towards sustainable water management and adaptation strategies in a changing world.

How to cite: Mey, J., Bookhagen, B., Haerter, J., Feulner, G., and Wagener, T.: The Potsdam WaterHub - Research, Networking, Training and Outreach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9213, https://doi.org/10.5194/egusphere-egu26-9213, 2026.

EGU26-9675 | ECS | Orals | EOS1.1

From Landscape to Geohazard: Assessing volcanic hazard communication in Tenerife geosites. 

Olaya Dorado, Thais Siqueira, Juana Vegas, Inés Galindo, David Sanz-Mangas, Lucía Sáez-Gabarrón, Rayco Marrero, Vanesa Burgos, Itahiza Domínguez-Cerdeña, Ruben López Díaz, and Carmen Romero

Volcanic landscapes attract millions of visitors annually, drawn by their unique geodiversity. However, these environments present a dichotomy: they are significant economic resources, but they also pose potential hazards for both residents and tourists. Effective risk mitigation also requires preparedness, integrating hazard awareness directly into the visitor experience. A key challenge lies in designing communication strategies that maintain scientific rigor and inform about active processes without generating unnecessary alarmism. 

This issue is particularly pertinent in Tenerife, which is currently under a volcanic unrest, and hosts 21 volcanic geosites listed in the Spanish National Inventory of Geosites (IELIG, open access https://info.igme.es/ielig/), 12 of which are located within active volcanic areas. Despite these numbers, the representation of volcanic risk in public outreach materials at these sites remains largely unassessed. Consequently, both residents and the over 7 million annual tourists may lack essential knowledge regarding the island’s eruptive potential, associated hazards, and the critical role of scientific monitoring in ensuring their safety.

This study evaluates eight key geosites in Tenerife, selected within the framework of the “Canary Islands: Destination of Volcanoes” project for their relevance to active volcanism. We conducted an evaluation of available outreach materials (including in-situ signage, printed brochures, and official web portals) based on three core criteria: i) the scientific accuracy and currency of the data presented; ii) the thematic scope (e.g., geological formation, environmental values, active volcanic processes, etc); and iii) the presence of specific information regarding volcanic hazards and risk management (preparedness, monitoring, and emergency protocols).

Beyond assessment, we aim to bridge the identified gaps by integrating risk communication strategies directly into the project’s outreach materials. This entails updating existing materials and embedding volcanic hazard modules into the project's newly developed materials and training courses for nature guides. By ensuring a balanced narrative that educates without inciting alarm, we propose a model of resilient geotourism where risk preparedness is intrinsic to the visitor experience, thereby enhancing general knowledge of active volcanic processes among both residents and tourists.

Sub-Project 1 ‘Canary Islands, destiny of Volcanoes’ (led by IGME-CSIC) is funded by PROMOTUR SA through Next Generation EU funds, PRTR. 2024krQ00nnn, carried out within the framework of the agreement between Promotur Turismo Canarias, S.A. and the CSIC, Univ. of La Laguna, Fundación Canaria General of the Univ. of La Laguna, and Univ. of Las Palmas de Gran Canaria.

How to cite: Dorado, O., Siqueira, T., Vegas, J., Galindo, I., Sanz-Mangas, D., Sáez-Gabarrón, L., Marrero, R., Burgos, V., Domínguez-Cerdeña, I., López Díaz, R., and Romero, C.: From Landscape to Geohazard: Assessing volcanic hazard communication in Tenerife geosites., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9675, https://doi.org/10.5194/egusphere-egu26-9675, 2026.

EGU26-10122 | ECS | Posters on site | EOS1.1

The “Next-Gen COP” as a tool for communicating climate change and catalyze solutions from high school students 

Francesca Munerol, Lara Polo, edoardo cremonese, Martina Leone, Giulia Blandini, Marta Galvagno, Chiara Guarnieri, Sofia Koliopoulos, Martina Lodigiani, Maddalena Nicora, Alessandro Benati, Fabrizio Sapone, Paolo Pogliotti, Gianluca Filippa, Federico Grosso, Sara Favre, Francesco Avanzi, and Margherita Andreaggi

The “Next-Gen COP”, developed by CIMA Research Foundation in collaboration with ARPA Valle d’Aosta and Fondazione Montagna Sicura, is an innovative climate-education programme designed to empower secondary-school students with the knowledge, skills, and agency needed to engage meaningfully in climate action. By simulating the negotiation dynamics of the UNFCCC Conference of the Parties, the initiative integrates scientific literacy, sociopolitical understanding, and participatory decision-making into a single experiential learning pathway. 

Launched in 2023 within the RESERVAQUA project, the “Next-Gen COP” focuses on climate-induced water challenges - drought, competing uses, and resource conflicts - issues that strongly affect Alpine and Mediterranean regions. The programme combines multiple pedagogical components: 

  • scientific training on the physical and legal-political dimensions of climate change; 
  • collaborative problem-solving, where students design water-management strategies inspired by the Sustainable Development Goals; 
  • dialogue with experts, enabling learners to refine proposals through evidence-based reasoning; 
  • Peer-to-peer communication, through poster sessions and public presentation; 
  • a final negotiation simulation, mirroring COP procedures, including amendments, consensus-building, and voting. 

This structure allows students to develop not only climate knowledge, but also key competences highlighted in the session,such as systems thinking, critical analysis, negotiation, and civic engagement. Indeed, the process culminates in a “Next-Gen Charter”, containing ten adaptation and mitigation proposals, formally presented to local policymakers, thereby linking classroom learning to real-world governance. 

The first edition in Valle d’Aosta involved around 150 students and demonstrated the programme’s capacity to foster climate agency, strengthen understanding of water-related risks, and promote inclusive, community-oriented climate action. The model is now being replicated in Liguria and Trento-Bolzano, expanding its reach and enabling comparative insights across diverse socioenvironmental contexts. 

The “Next-Gen COP” offers a scalable and transferable approach to climate change education, showing how experiential, participatory, and policy-oriented learning can empower young people to contribute actively to climate resilience at local and global scales. 

How to cite: Munerol, F., Polo, L., cremonese, E., Leone, M., Blandini, G., Galvagno, M., Guarnieri, C., Koliopoulos, S., Lodigiani, M., Nicora, M., Benati, A., Sapone, F., Pogliotti, P., Filippa, G., Grosso, F., Favre, S., Avanzi, F., and Andreaggi, M.: The “Next-Gen COP” as a tool for communicating climate change and catalyze solutions from high school students, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10122, https://doi.org/10.5194/egusphere-egu26-10122, 2026.

EGU26-10123 | Orals | EOS1.1

The Italian Citizen Science Observatory: a growing association open to collaboration to foster public participation and education in water research Europe-wide 

Luisa Galgani, Bruna Gumiero, Francesco Di Grazia, Marco Cossu, and Steven A. Loiselle

The Italian Citizen Science Observatory, established in 2016, seeks to encourage public involvement in science by turning citizens into active contributors to scientific research. Its objective is to implement Citizen Science to strengthen collaboration between researchers and civil society, building an increasingly close relationship between science and the wider community. The Observatory focuses on monitoring and safeguarding the health of freshwater ecosystems—such as rivers, lakes, streams and wetlands—on which everyone relies, as well as the surrounding riparian areas. One of the pillars of the Observatory's mission is education, with a strong focus on schools as key environments for the development of scientific literacy, environmental awareness, and active citizenship. Schools are recognized not only as places of learning, but also as catalysts for cultural change, capable of amplifying Citizen Science practices within families and local communities. Through practical monitoring and inquiry-based learning activities, students become active observers of their local freshwater ecosystems and ambassadors for sustainable behavior.

The Observatory actively promotes peer education approaches, encouraging the exchange of knowledge between students, teachers, citizens, and researchers. This horizontal learning model improves engagement, empowers young people as science communicators, and strengthens intergenerational dialogue on environmental protection.

A recent accomplishment of the Observatory is the development of the RiVE (Riparian Vegetation) methodology as a Citizen Science tool for monitoring riparian zones. RiVE assesses riparian zone ecological health by the engagement of local communities in tracking plant diversity and ecosystem functions. This approach highlights the importance of these biodiversity-rich corridors for river health and management, often contrasting with fixed-width buffer approaches. The Observatory serves as the first Italian hub of the Earthwatch FreshWater Watch program, defining and sharing best practices for data collection and creating new tools whenever required. It also runs pilot initiatives in protected areas and works more broadly with local environmental bodies and associations.

We here present the activities undertaken at the Observatory, from building Citizen Science initiatives and communities to training both citizens, schoolteachers, school children and students, policy makers and researchers, encouraging the active engagement of all society actors in scientific endeavours and aquatic ecosystems management and protection.

At EGU we hope to spark new collaboration opportunities and expand the Observatory network to foster the co-creation and management of Citizen Science projects across Europe and beyond.

https://www.osservatoriocitizenscience.org/home/

How to cite: Galgani, L., Gumiero, B., Di Grazia, F., Cossu, M., and Loiselle, S. A.: The Italian Citizen Science Observatory: a growing association open to collaboration to foster public participation and education in water research Europe-wide, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10123, https://doi.org/10.5194/egusphere-egu26-10123, 2026.

EGU26-10224 | Posters on site | EOS1.1

Open Science Network: Distributed social infrastructure for open scientific discussion 

Jorge Saturno, Ivan Minutillo, Mayel de Borniol, Pierre Boudes, Nicolas Fressengeas, and Ulrike Hahn

Scientific conversations that once took place on Twitter have scattered to other platforms, such as LinkedIn and Bluesky. Like Twitter, these services operate as walled gardens, limiting access for unregistered users. Furthermore, identity verification and public recognition have become paid services that lack reliability and oversight.

Thanks to a W3C-standardized protocol called ActivityPub, the same one behind Mastodon, open and distributed social feeds, where users from different servers can read and interact, are already available. Using open protocols is the best way to enable scientific communication that both peers and the general public can trust.

The Open Science Network (https://openscience.network/) is designing and deploying a software for federated scientific communication. The app uses Bonfire's open-source framework and the ActivityPub protocol as a backbone. The goal is to create federated digital spaces in which researchers and institutions have complete control over their data, including their conversations and networks. Universities can host their own instances while being interconnected with a global network of scientific communities. Discussions can become citable, FAIR objects with DOIs. Publications are enriched with metadata and collaborative tools.

The Open Science Network is co-designed with researchers, scientific communities, and open science advocates who understand that scientific communication tools shape science itself. Platforms that prioritize engagement over accuracy cannot facilitate reliable scientific communication. The software provides ORCID authentication and Zenodo repository archiving for social posts. Planned features include custom peer review, multiple trust signal workflows, semantic data linking, a framework for experimenting with new forms of scientific communication, proper and verified attribution, federated groups, knowledge management and curation tools, long-term preservation, and space for inventing features not included in this list.

How to cite: Saturno, J., Minutillo, I., de Borniol, M., Boudes, P., Fressengeas, N., and Hahn, U.: Open Science Network: Distributed social infrastructure for open scientific discussion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10224, https://doi.org/10.5194/egusphere-egu26-10224, 2026.

EGU26-10625 | ECS | Orals | EOS1.1

From Network to Ecosystem: Reflecting on Early Career–Led Science Communication through APECS 

Deniz Vural, Alice Guzzi, Anastasia Deyko, Pratik Kad, Sophie Dupont, Hugo Guimaro, and Sebastian Maria Karl Heinrich Kopf

Science communication is often framed as a unidirectional transfer of knowledge from scientists to society. For early career researchers (ECRs), however, it also plays a crucial role in building community, fostering belonging, and co-creating knowledge across disciplines, cultures, and career stages. The Association of Polar Early Career Scientists (APECS) offers a case study on how science communication can function as a long-term, community-driven ecosystem rather than a series of one-off outreach activities.

APECS is a global, ECR-led organization supporting early career researchers working in polar and cryosphere science, founded in 2007 following the momentum and international collaboration fostered by the Fourth International Polar Year (IPY-4). Although not always labelled explicitly as “science communication”, many of APECS’ core activities involve communicating science and co-creation of scientific knowledge within ECR communities and beyond. The activities include engagement with policymakers, Indigenous Peoples’ organizations, local communities, educators, and the wider public. Through programmes, workshops, leadership development, and community-led initiatives, APECS supports ECRs in developing skills in outreach, public engagement, inclusive communication, and collaborative knowledge production, contributing to long-term capacity building within polar and cryosphere research communities.

This contribution reflects on APECS’ science communication practices through three key questions. First, how can science communication spark joy and foster emotional connection? APECS emphasizes storytelling, peer mentoring, and shared experiences, from informal networking spaces to collaborative events, that humanize polar science by helping ECRs connect emotionally with their research and with peers. These approaches are particularly important in polar research, where geographic isolation, logistical barriers, and short-term contracts can limit a sense of community.

Second, how can co-creation be meaningfully embedded within scientific communities? APECS operates through bottom-up leadership, with initiatives proposed, led, and shaped by ECRs themselves. This structure enables co-creation across disciplines, cultures, and regions, and fosters dialogue between natural scientists, social scientists, and knowledge holders from diverse backgrounds.

Finally, how can the impacts of science communication be assessed over time? Rather than focusing solely on short-term metrics, APECS reflects on longer-term indicators such as sustained engagement, leadership development, capacity building, career trajectories, and continued participation in interdisciplinary and societal dialogues, dimensions that are often overlooked in traditional evaluations of science communication.

By reflecting on both successes and challenges, this contribution highlights lessons learned from long-term ECR engagement and offers insights for designing inclusive, community-based science communication initiatives that strengthen both scientific practice and its relationship with society.

How to cite: Vural, D., Guzzi, A., Deyko, A., Kad, P., Dupont, S., Guimaro, H., and Kopf, S. M. K. H.: From Network to Ecosystem: Reflecting on Early Career–Led Science Communication through APECS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10625, https://doi.org/10.5194/egusphere-egu26-10625, 2026.

EGU26-10850 | Posters on site | EOS1.1

Communicating geoscience on social media: Harnessing the short video format 

Laura Säilä-Corfe, Anna Sartell, and Samuli Siltanen

Short videos, which provide concise, clearly articulated, and engaging content on a wide variety of topics are among the most prominent formats on platforms such as YouTube, Instagram, Facebook, LinkedIn, and TikTok. The short video format is particularly well suited to the dissemination of scientific knowledge and research findings to non-specialist audiences, offering researchers a valuable means of broad societal engagement.

 

The University of Helsinki Faculty of Science trains and motivates researchers to adopt and apply the short-video format for science communication by offering the How to Make a Science Video course, jointly by the journalism program at Haaga-Helia University of Applied Sciences. The course, offered annually, is led by experienced science video producers and journalism professionals. Participants work in mixed teams comprising researchers at different career stages from master’s students to professors—together with journalism students from Haaga-Helia. The course covers, among other topics:

  • Developing an initial idea into an engaging video
  • Popularizing scientific concepts
  • Creating effective educational videos
  • Writing persuasive scripts
  • Speaking and performing on camera
  • Shooting and editing high-quality videos using only a smartphone
  • Selecting appropriate channels and strategies for publication

Each team produces a science video of up to two minutes duration, which is published at the conclusion of the course on the YouTube channels of both institutions.

 

As part of the course in 2024, we set out to make an educational video about ancient volcanism in southern Finland.  Around 1.9 billion years ago, there was a volcanic island arc in southern Finland and outcrops of these rocks can be found in, for example, the Helsinki region. We filmed in some of these locations, interviewed a local expert and author of a book on this topic, and included an animation made by a close collaborator on how the volcanic rocks formed in our 2-minute video. Our final Youtube video and the process of making it are here used as an example of all the methods and skills we learned on the How to make a science viodeo course.

How to cite: Säilä-Corfe, L., Sartell, A., and Siltanen, S.: Communicating geoscience on social media: Harnessing the short video format, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10850, https://doi.org/10.5194/egusphere-egu26-10850, 2026.

Climate change is placing increasing pressure on global food systems that are vital to human survival. Understanding the interconnections between food (including seeds), agriculture, and climate is crucial for building resilient and sustainable futures. However, science communicators often struggle to translate complex food–climate concepts for non-specialist audiences. Effective engagement thus requires messages that are accurate, relatable, and connected to daily life.

Drawing on collaborative outreach programmes and public lecture series on food and climate, this contribution illustrates how interactive formats, such as climate-friendly cooking workshops, field visits, and seed-focused learning, to deepen understanding, stimulate curiosity, and foster critical thinking. These initiatives bridge disciplinary silos while engaging diverse audiences, including students, educators, and members of the public. Through enhanced dialogue, reflection, and experimentation, they demonstrate how science communication empowers individuals to make informed food choices, advancing both science literacy and community action towards sustainable food systems.

How to cite: Mok, H.: Communicating Food and Climate: The Role of Science Communication for Engagement  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11213, https://doi.org/10.5194/egusphere-egu26-11213, 2026.

EGU26-11214 | ECS | Orals | EOS1.1

Science communication in Greenland: Experiences from the Kalaallit Nunaat Caves and Climate Outreach Project (KINDLE) 

Lena K. Anders (neè Friedrich), Gina E. Moseley, Oline Petersen, Kristian Kaspersen, and Kerim Hestnes Nisancioglu

Effective science communication is essential for building trust between researchers and society, particularly in regions where environmental change is rapid and directly affects local communities. In Greenland, the National Research Strategy emphasises inclusive, community-centred research and the active involvement of Greenlanders in scientific processes. Within this context, the Kalaallit Nunaat Caves and Climate Outreach Project (KINDLE) was developed as a science communication initiative linked to the Greenland Caves Project, which investigates palaeoclimate, cave systems, and geological processes in northern Greenland.

KINDLE was designed to explore ways of strengthening connections between research and society by working with Greenlandic communities to share scientific work in accessible formats, support locally grounded engagement with cave environments, and encourage long-term participation in cave exploration and research. The project employed a range of communication approaches in multiple languages, including an interactive exhibition, micro-documentaries, hands-on workshops for children, public presentations with open Q&A sessions, and practical caving skills workshops for adults. These activities were hosted during a one-month residency at the ILLU Science & Art Hub in Ilulissat, part of the Climate Narratives initiative, which promotes climate communication through diverse forms of storytelling.

Based on the experiences from the residency, we reflect on lessons that may be informative for other Earth science contexts, including the value of storytelling that emphasizes how science is done over specific results, the importance of local partnerships and trusted venues, and the need to approach science communication as an evolving, collaborative practice. The project illustrates how science communication can move beyond dissemination toward participation, with the long-term aim of enabling local communities to engage with, contribute to, and potentially lead future research and exploration initiatives.

How to cite: Anders (neè Friedrich), L. K., Moseley, G. E., Petersen, O., Kaspersen, K., and Nisancioglu, K. H.: Science communication in Greenland: Experiences from the Kalaallit Nunaat Caves and Climate Outreach Project (KINDLE), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11214, https://doi.org/10.5194/egusphere-egu26-11214, 2026.

EGU26-11554 | Posters on site | EOS1.1

Geology for All: Engaging the Public with a Simplified and Accessible Geological  Map of Rome 

Giuditta Radeff, Silvana Falcetti, Deborah Maceroni, Patrizio Petricca, Matteo Simonetti, Stefano Urbani, and Chiara D'Ambrogi

Geological maps are fundamental tools in geoscientific research and play a critical role in land-use planning, risk assessment and resource management. However, their complexity, interdisciplinary nature and dense data content often make them difficult to interpret for non-specialist audiences. Consequently, their potential as tools for science communication remains largely untapped.

To foster greater public involvement in Earth sciences and to increase awareness of the influence of geology on everyday life, and drawing inspiration from the 2022 educational geological map of the Paris region produced by the French Geological Survey (BRGM) in the series of geological maps for educational purposes (https://www.brgm.fr/en/news/news/three-new-geological-maps-educational-purposes), we developed a prototype simplified geological map derived from the Geological Map of Sheet 374 – Rome (CARG Project, Geological Survey of Italy).

The simplified geological map of Rome is designed to reach a broad and diverse audience, from young students to tourists, citizens, policymakers and stakeholders, encompassing a wide range of ages, languages, educational backgrounds and abilities. To achieve this, the product combines scientific accuracy with visual engagement, presenting content in at least two languages (Italian and English), with simple explanations for beginners and additional information for those wishing to explore the topic in more depth.

Special attention was given to the design: map colours were chosen to be colour-blind friendly, and a freely available font was adopted to mitigate common symptoms of dyslexia (https://opendyslexic.org/). Efforts are ongoing to develop a version accessible to visually impaired users.

The prototype is flexible and replicable, capable of being adapted to other regions and geological contexts. It integrates a simplified geological map, a geological cross-section, a geological timescale and an intuitive, visually appealing, legend, providing a clear representation of the relationships among geological structures, georesources and geo-hazards in a highly urbanized environment.

This project represents a science communication experiment aimed at translating authoritative, technically oriented geological maps into simplified, visually engaging products that maintain scientific rigor while enhancing accessibility, understanding and public engagement with Earth sciences.

How to cite: Radeff, G., Falcetti, S., Maceroni, D., Petricca, P., Simonetti, M., Urbani, S., and D'Ambrogi, C.: Geology for All: Engaging the Public with a Simplified and Accessible Geological  Map of Rome, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11554, https://doi.org/10.5194/egusphere-egu26-11554, 2026.

EGU26-12132 | Orals | EOS1.1

Engaging young audiences in climate change: moving beyond fear through active science communication 

Marta Galvagno, Chiara Guarnieri, Sofia Koliopoulos, Paolo Pogliotti, Gianluca Filippa, Federico Grosso, Nicolas Lozito, Francesca Munerol, Sara Favre, Edoardo Cremonese, Alessandro Benati, Simone Gottardelli, Fabrizio Sapone, and Francesco Avanzi

Science communication is not only about conveying scientific findings, but also about fostering dialogue, understanding, and engagement among non-specialist audiences. In the context of climate change, narratives emphasizing catastrophic outcomes and individual responsibility can unintentionally foster fear, anxiety, and disengagement, particularly among younger audiences. Such fear-based communication may contribute to forms of inactivism, in which concern does not translate into action but instead leads to emotional paralysis. Communicating “efficiently” therefore means avoiding both denialism and doomism, as well as individualism, while preserving scientific accuracy and urgency.

In recent years, public trust in science has been questioned in many countries, influenced by political polarization, the spread of misinformation, skepticism toward scientific credibility, and contested roles of scientists in public decision-making.  In this context, scientists have a social responsibility not only to convey accurate information but also to frame the scientific message in ways that empower understanding and collective responses.

In this contribution, we reflect on climate communication strategies that move beyond frontal, passive teaching toward active and participatory engagement. Relying on outreach activities in secondary schools, we present results from questionnaires delivered before and after climate science lessons, with a specific focus on changes in students’ emotional responses and perceptions. The findings indicate that participatory approaches, such as interactive discussions, problem-solving simulations, and solution-oriented framing, can reduce anxiety and inactivism, while strengthening understanding, motivation to take action, and trust in scientific knowledge.

We argue that communicating climate change without catastrophism but emphasizing achievable pathways for action is not a dilution of problem urgency, but a necessary step toward enabling rational and hopeful societal responses to global challenges, particularly among younger generations, and in times of converging crises.

How to cite: Galvagno, M., Guarnieri, C., Koliopoulos, S., Pogliotti, P., Filippa, G., Grosso, F., Lozito, N., Munerol, F., Favre, S., Cremonese, E., Benati, A., Gottardelli, S., Sapone, F., and Avanzi, F.: Engaging young audiences in climate change: moving beyond fear through active science communication, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12132, https://doi.org/10.5194/egusphere-egu26-12132, 2026.

EGU26-12150 | Posters on site | EOS1.1

Allin-Wayra: advancing equitable and transparent use of small sensors through a global community of practice 

Sebastian Diez, Nicole Cowell, Eliani Ezani, Miriam Chacón-Mateos, Àlex Boso, John Richard Hizon, and Kwabena Fosu-Amankwah

Small sensor technologies are rapidly expanding access to atmospheric observations, offering new opportunities to complement regulatory air-quality monitoring and to address persistent data gaps. However, the benefits of these technologies are unevenly distributed, and their effective use is constrained by variability in data quality, limited transparency in data processing, and unequal access to technical capacity and guidance. These challenges are particularly acute in low- and middle-income regions, where monitoring infrastructure and institutional resources remain limited.

The “Allin-Wayra: Small Sensors for Atmospheric Science“ (https://igacproject.org/activities/allin-wayra-small-sensors-atmospheric-science) initiative was established within the International Global Atmospheric Chemistry (IGAC) Project to build a global, inclusive community of practice around responsible sensor use, with a strong focus on equity, capacity building, and transparency. Core activities include community workshops, an international webinar series, conference sessions,  the co-development of open-access repositories and guidance resources, and targeted efforts to improve accessibility and dissemination. 

This presentation reflects on early lessons learned from launching and coordinating a distributed global community, highlighting strategies for inclusive engagement, cross-regional and cross-disciplinary co-creation and mechanisms to sustain participation beyond individual projects, while gaining insights from other sensor communities of practice. We discuss practical challenges in balancing scientific rigor with accessibility, fostering trust in emerging technologies, whilst encouraging cross-sectoral collaboration (policy, business, non-profit and scientists). By sharing these experiences, we aim to identify how community-driven governance can co-create more equitable and impactful environmental research practice and decision-making.

How to cite: Diez, S., Cowell, N., Ezani, E., Chacón-Mateos, M., Boso, À., Hizon, J. R., and Fosu-Amankwah, K.: Allin-Wayra: advancing equitable and transparent use of small sensors through a global community of practice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12150, https://doi.org/10.5194/egusphere-egu26-12150, 2026.

EGU26-12383 | Orals | EOS1.1

Access, verification, and trust in extreme weather events communication: age and discipline matter 

Tatiana Izquierdo, Beatriz Catalina-García, Carlos Sánchez-García, María del Carmen García-Galera, and Manuel Abad

Effective communication of extreme weather events (EWEs) requires understanding how audiences access, evaluate, and respond to information, which is critical for improving science communication strategies on climate-related risks. To examine these processes among young adults, we conducted a structured survey administered to undergraduate students at two Spanish universities (Rey Juan Carlos University and Autonomous University of Madrid). The survey, disseminated online during regular teaching periods, used voluntary participation and collected 746 responses across diverse academic programmes. It comprised multiple-choice and Likert-scale items covering interest in specific EWEs (e.g., intense rainfall, heatwaves, floods), primary modes of information access (intentional search, incidental exposure, or balanced patterns), verification behaviours, perceived prevalence of fake news in both searched and unsolicited content, trust in ten different media channels, and self-assessed ability to detect misinformation. Differences were assessed using descriptive statistics and comparative analysis.

Age-tercile analysis using quantile cuts (18; 18–20; >20) shows stable but informative gradients. Verification frequency (1–5) rises slightly with age (2.99 → 2.96 → 3.05), while event-specific interest (1–4) remains high and broadly flat (3.13 → 3.11 → 3.16). Trust in social platforms increases marginally (1.92 → 2.07 → 2.08), whereas trust in traditional outlets and science-oriented sources stays comparatively stable (traditional 3.28–3.37–3.35; science 4.04–4.09–4.08). Self-reported ability to detect misinformation (1–7) shows a small step-down across terciles (4.79 → 4.71 → 4.66). For access patterns, the share of balanced access (search + incidental) is higher from the middle tercile onward (52.9% → 61.4% → 58.6%), with a corresponding reduction in purely incidental exposure (43.6% → 36.0% → 38.7%), while intentional search only remains low (3.6% → 2.6% → 2.7%). Consistently across terciles, students perceive more fake news in incidental flows than in self-searched content (+1.11, +1.00, +1.18).

Comparing academic disciplines (science vs. communication) reveals clear structural contrasts. Students in scientific programs report higher general interest in EWEs (3.56 vs 3.24) and slightly greater event-specific interest (3.17 vs 3.09), alongside marginally lower verification frequency (2.98 vs 3.03). Self-reported ability to detect misinformation also trends higher in science (≈4.80 vs 4.62). Trust architectures differ markedly: communication students show stronger confidence in traditional media (3.57 vs 3.15), while science lean toward science-oriented sources (4.11 vs 4.00). Trust in social platforms remains low across both groups, though slightly higher in communication (2.05 vs 1.99). These patterns underscore the need for differentiated strategies: technical and data-rich content for science students, and journalistic narrative formats for communication, complemented by platform-specific adaptations to maintain credibility and engagement.

These findings suggest practical actions to improve communication: ensure multi-platform dissemination with consistent core messages; highlight transparent sourcing and authoritative voices; adapt formats by age (visual checklists for younger students, data-rich dashboards for older ones); and tailor content to disciplinary expectations (technical and quantitative for science, journalistic narrative for communication). Aligning formats and channels with audience information habits can enhance comprehension, reduce misinformation, and support informed decision-making during EWEs.

How to cite: Izquierdo, T., Catalina-García, B., Sánchez-García, C., García-Galera, M. C., and Abad, M.: Access, verification, and trust in extreme weather events communication: age and discipline matter, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12383, https://doi.org/10.5194/egusphere-egu26-12383, 2026.

EGU26-12641 | ECS | Orals | EOS1.1

Community outreach using positive sensory experiences: A taste of climate change 

Alex Valach, Christine Jurt, and Sébastien Boillat

Communicating scientific advances and their impacts on society in an accessible manner is an inherent requirement of those engaged with science. Sensitising the public on climate change topics typically relies on rational discourse and the sharing of factual details. However, our first response to novelty, especially in stressful environments is usually emotional and with increasing political polarization, the individual’s priming, environment and beliefs heighten this response to the point of confrontation, avoidance and even denial. One way to potentially mitigate existing negative emotional biases is to approach the topic using a positive emotional experience that is widely shared regardless of identity, such as consuming food and drink.

Our project supported by an EGU public engagement grant consisted of small tasting events using locally produced and relevant food and drink items, which could be used as an example of how climate change is or will affect their production and consumption. Events can take on different formats depending on the situation and available resources, as well as allowing a wide range of consumables that can be adapted to the local community and values. Here we provide a brief overview of our activities and outline some implementation aids to support other groups or individuals interested in organizing their own events.

How to cite: Valach, A., Jurt, C., and Boillat, S.: Community outreach using positive sensory experiences: A taste of climate change, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12641, https://doi.org/10.5194/egusphere-egu26-12641, 2026.

EGU26-12649 | ECS | Posters on site | EOS1.1

Climate change communication from an inter- and transdisciplinary perspective – an example from ClimXtreme 

Paulina Fischer-Frenzel, Miriam Wagner-Jacht, Jens Grieger, Philip Lorenz, and Frank Kreienkamp

Climate change poses a scientifically highly complex issue due to being a process of global change with considerably different outcomes for different regions, underpinned by scientific uncertainty. The inherent nature of the ongoing climate change is dynamic and oftentimes non-linear, bearing the risk of increasing the likelihood (and exacerbating the intensity) of extreme weather events. Hence, the issue not only asks for climate research to be translated prior to being addressed towards audiences with few or no prior scientifical knowledge of the field, but for the climate knowledge also to be communicated in a precise, reliable and continuously updated – while comprehensible – manner.

ClimXtreme is a nationwide interdisciplinary project funded by the German Federal Ministry of Research, Technology and Space (BMFTR) and focusing on the improvement of the scientific understanding of extreme weather events in a changing climate as well as the transdisciplinary interaction with practice stakeholders.

As part of the research network of ClimXtreme II (2023-2026), the German Meteorological Service (Deutscher Wetterdienst, DWD) has designed and launched a communication tool in form of a knowledge base. Its aim is to compile, synthesise and communicate the research goals and results of the 25 subprojects from various disciplines towards different target groups (general public, practitioners, administrations, politics and the private sector). Thus, the knowledge base seeks to facilitate the dialogue between climate research and society and provide a tool for scientifically informed decision-making processes.

Furthermore, one main focus is illustrating the transdisciplinary interactions which have already been established within the project. In this regard, the platform serves as an example case for inter- and transdisciplinary demand-oriented communication and is hereby tackling challenges in climate change communication.

How to cite: Fischer-Frenzel, P., Wagner-Jacht, M., Grieger, J., Lorenz, P., and Kreienkamp, F.: Climate change communication from an inter- and transdisciplinary perspective – an example from ClimXtreme, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12649, https://doi.org/10.5194/egusphere-egu26-12649, 2026.

Indoor air quality is key due to the amount of time people spend indoors (approximately 80–90 % of their lives). However, understanding how time and activity dependent sources, as well as built environment characteristics, influence pollutant emissions and distributions remains very limited. Addressing these challenges, InAPI — an Indoor Air Pollution Inventory tool — has been developed using data synthesised from a comprehensive review of UK indoor air pollution research (Mazzeo et al., 2025; doi.org/10.5194/egusphere-2025-783). For the development of the InAPI tool, we have categorised existing literature by pollutant types, indoor environments, and activities, identifying significant knowledge gaps and offering an open-access database of typical pollutant concentrations and emission rates (Mazzeo et al., 2025; doi.org/10.1039/D4EA00121D). InAPI leverages this database to enable users to visualise indoor pollutant levels and emission characteristics across varied indoor settings. InAPI consolidates this evidence into a practical and easy-to-use tool which facilitates standardisation of IAQ measurement protocols and the creation of activity-based indoor emission inventories. By providing a robust platform for understanding indoor air pollutant dynamics, InAPI represents a significant step forward in advancing IAQ research given the transferability of the approach, supporting efforts to mitigate indoor air pollution with potential to inform policy initiatives. A key challenge to overcome is how to make this tool attractive and usable for non-experts and to ensure that the information is presented in a way that it can and will be used by policy makers and practitioners.

How to cite: Pfrang, C., Mazzeo, A., and Nazar, Z.: Developing an Indoor Air Pollution Inventory Tool to Visualise Activity-based Indoor Concentrations of Pollutants and Their Emission Rates for the Wider Community., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12812, https://doi.org/10.5194/egusphere-egu26-12812, 2026.

EGU26-12903 | Orals | EOS1.1

Visualising historical changes in air pollution with the Air Quality Stripes 

James McQuaid, Kirsty Pringle, Carly Reddington, Steven Turnock, Richard Rigby, Meruyert Shayakhmetova, Malcolm Illingworth, Denis Barclay, Neil Chue Hong, Ed Hawkins, Douglas Hamilton, and Ethan Brain

Air pollution poses a major public health risk, contributing to approximately 4.7 million premature deaths each year, the majority of which occur in low and middle-income countries. Effective public communication of air quality data is essential to drive policy action and address health inequalities, yet translating complex environmental data into an accessible format is always challenging.

This contribution presents findings from the Air Quality Stripes project (https://airqualitystripes.info/, Pringle KJ. et al, Geoscience Communication, 2025), which aims to raise public awareness and understanding of outdoor air pollution by visualising historical changes in fine particulate matter (PM₂.₅) in major global cities from 1850 to 2022*  in a clear and engaging manner. Inspired by the widely recognised Warming Stripes (https://showyourstripes.info/) images, the Air Quality Stripes project combined data from satellite observations and model simulations to create a continuous historical PM₂.₅ dataset, which was then displayed as a series of vertical stripes. 

The resulting visualisations reveal divergent pollution trends: there have been substantial improvements in air quality in many cities in Europe and North America, contrasted by persistently high or worsening pollution in parts of Asia, Africa, and South America. 

The project received significant public and media attention, including coverage in major national newspapers and broadcast media, demonstrating a strong appetite for accessible representations of air pollution data. They have also been used by a major philanthropic funder which funds observational networks to highlight gaps in global air quality data, especially in developing nations. In addition, major advocacy groups such as the C40 cities program are also using the images in their visualisation toolkit as part of their campaign for transparent air quality data to improve public health and policy.

What lessons have been learned?

Beyond describing the Air Quality Stripes visualisations, this contribution reflects on broader lessons for environmental data communication, drawing on audience engagement, media uptake, and practitioner feedback including:

  • Collaboration with visual experts. The colour palette was developed with a design expert, drawing on imagery of air pollution to create a tangible link between colour and pollution.
  • Informal feedback and review. Iterative feedback from colleagues, friends, and family helped improve the images; for example, early versions showed concentrations only, and feedback led us to add indicative labels (e.g. “good”, “poor”) to provide health-related context.
  • City-specific focus. We chose to present images from individual cities as regional averaging would blur historical trends, but this city focus was popular with viewers as it allowed the viewer to connect with the information on a more tangible and often personal level.
  • Selected annotations. Narrative annotations on a subset of images made the data more relatable, providing context and highlighting significant points. They also helped viewers better understand the overall structure of the images.

Lessons from the Air Quality Stripes project apply broadly to science communication, highlighting the value of interdisciplinary collaboration, iterative engagement with non-experts, and careful use of colour, context, and narrative. These insights extend beyond the project to inform environmental data visualisation and public communication more widely.

How to cite: McQuaid, J., Pringle, K., Reddington, C., Turnock, S., Rigby, R., Shayakhmetova, M., Illingworth, M., Barclay, D., Chue Hong, N., Hawkins, E., Hamilton, D., and Brain, E.: Visualising historical changes in air pollution with the Air Quality Stripes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12903, https://doi.org/10.5194/egusphere-egu26-12903, 2026.

EGU26-13519 | Posters on site | EOS1.1

Sharing science on the road: Bringing a traveling exhibit on extreme weather and community resilience to Alaska through community and private sector partnerships 

Daniel W. Zietlow, Rebecca Haacker, Becca Hatheway, Patricia Montaño, Auliya McCauley-Hartner, Evan Portier, John Smelter, Emily Snode-Brenneman, and Amy Stevermer

From professional radiosonde data to information from a backyard rain gauge, observation is key to understanding extreme weather and our local environment. Resilient Earth, Resilient Communities, a traveling exhibit collaboratively designed by the Center of Excellence for Education, Engagement & Early-Career Development (EdEC) at the U.S. National Science Foundation National Center for Atmospheric Research (NSF NCAR) and the University Corporation for Atmospheric Research’s Center for Science Education (UCAR SciEd), explores how we use this foundational concept of observation to gather information on extreme weather patterns and subsequent impacts on local environments in order to build more resilient communities. Since 2019, the exhibit has traveled to 19 locations across the United States, including public libraries, cultural centers, and universities. With each host, we co-design one exhibit display of content to contextualize the exhibit within specific extreme weather events experienced by the host community and adaptation strategies being employed by community members. In 2025, the exhibit team collaborated with hosts across Alaska to bring the exhibit to five different locations. Additionally, we partnered with a private company to bring a smaller version of the exhibit to passengers on an expedition cruise ship traveling throughout coastal Alaska. In this presentation, we address our co-design process for collaborating with and engaging communities and the private sector. We will also discuss results from a recent evaluation of the effectiveness of the exhibit in sparking dialog and creating emotional connections to the content, as well as provide actionable insights to designing a traveling exhibit.

How to cite: Zietlow, D. W., Haacker, R., Hatheway, B., Montaño, P., McCauley-Hartner, A., Portier, E., Smelter, J., Snode-Brenneman, E., and Stevermer, A.: Sharing science on the road: Bringing a traveling exhibit on extreme weather and community resilience to Alaska through community and private sector partnerships, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13519, https://doi.org/10.5194/egusphere-egu26-13519, 2026.

Rainfall is a familiar phenomenon for most people and is often perceived as a constraint. Yet, it usually receives little attention, as daily activities take priority. As rainfall and hydrology scientists, we seek to engage the general public and improve understanding in a field that is often affected by misinformation. More broadly, our goal is to stimulate curiosity and awareness of the surrounding geophysical environment.

To contribute to this effort, we designed and implemented a series of multisensory experiences centered on rainfall, guided by three main objectives: (i) to actively engage people with geoscience topics by encouraging them to observe their environment; (ii) to offer a simple and enjoyable moment that allows them to focus on geophysical phenomena; and (iii) to provide new knowledge about rainfall. Regarding this last objective, sensory involvement is a powerful tool for enhancing learning and memory.

We proposed three simple experiences that require no material other than rainfall itself and an open mind, and that conveys clear take-home messages. The three experiences are: feeling raindrops and their sizes on the hand or face while walking; listening to rain falling on different surfaces (such as a tent, umbrella, or metal sheet); and observing rainfall near a lamppost at night. The first highlights the variability of drop sizes, the second illustrates the temporal variability of rainfall, and the third reveals the combined temporal variability of rainfall and wind. Participants are invited to read short instructions before, and to fill out an open-ended form to report their sensations and observations.

The feedback collected for more than 60 experiences carried out in more than 5 different countries will be presented. Disparities of feeling between the three experiences will be presented.

How to cite: Gires, A. and Dallan, E.: Enhancing awareness of the geophysical environment through a multisensory rainfall experience, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14749, https://doi.org/10.5194/egusphere-egu26-14749, 2026.

EGU26-14937 | Posters on site | EOS1.1

Groundbreaking Science Discoveries and Successes enabled by ESA Earth Observation Satellites 

Maurice Borgeaud, Jonathan Bamber, Anny Cazenave, Yann Kerr, Michaela Hegglin, Marta Marcos, Christian Massari, Johanna Tamminen, Chris Rapley, Jonas L'Haridon, and Courtney Allison

The presentation will introduce a brochure (see reference below) that was prepared by the Earth Science Panel of the European Space Science Committee, which describes twelve groundbreaking science examples enabled by Earth observation satellites, representing the four main thematic domains of Earth sciences, namely: atmosphere, polar regions, ocean, and land. The different examples highlight the value across the Earth sciences of Earth Observation satellite missions, how they have resulted in transformative scientific breakthroughs, and their value to society and human endeavour.

Taking note that ESA is already very active in the communications of EO results, https://www.esa.int/Applications/Observing_the_Earth, the aim it to produce a simple and easy to understand document that can convincingly demonstrate the huge science and societal benefits brought by ESA EO satellites. The document provides 12 examples clearly identifying the discoveries enabled by EO satellites.  Most examples are based on ESA missions (ERS-1, ERS-2, ENVISAT, Earth Explorers) and European Commission Copernicus programme (Sentinels), but other sources of data from European national missions and NASA are used.

The approach for the preparation of this document was driven by an ambition to translate the details and results of landmark scientific breakthroughs to a policy-oriented audience through the employment of concise, clear, and approachable language. To further aid in understanding, the text was accompanied by impactful and sharp graphics generated in collaboration between the scientists, communication experts, and professional graphic designers.

The presentation will describe how the document was conceived, the selection process to arrive at the 12 examples, and the satellite data used. Special attention will be also given on the process to convert scientific results published from highly ranked journals to easily understandable text and graphics which make the core of the document. Lessons learned on the process will be reported and some of the examples of the brochure will be detailed in the presentation.

This new perspective could act as a template for future promotion of space agency scientific excellence and value.

 

Reference:

Borgeaud, M., Bamber, J., Cazenave, A., Hegglin, M., Kerr, Y., Marcos, M., Massari, C., Tamminen, J., Rapley, C., L’Haridon, J. and Allison, C., Earth Observation Groundbreaking Science Discoveries, ESA publication, 2025, https://doi.org/10.5270/ESSC-ESA-EO-Groundbreaking-Science-2025, available for download at https://www.essc.esf.org/2025/01/21/news-eo-brochure/.

 

 

How to cite: Borgeaud, M., Bamber, J., Cazenave, A., Kerr, Y., Hegglin, M., Marcos, M., Massari, C., Tamminen, J., Rapley, C., L'Haridon, J., and Allison, C.: Groundbreaking Science Discoveries and Successes enabled by ESA Earth Observation Satellites, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14937, https://doi.org/10.5194/egusphere-egu26-14937, 2026.

EGU26-15455 | Orals | EOS1.1

Learning, creating, and sharing: A science communication framework for water and climate education 

Lisa Gallagher, Jasmine Pinchinat, Mario Soriano, and Reed Maxwell

Since 2015, the Integrated GroundWater Modeling Center has engaged diverse audiences in water and climate science through community education and outreach programs including STEM fairs, university courses, teacher workshops, and week-long camps for high school students. Across these varied contexts, science communication has served as a consistent throughline, informing both how participants learn scientific content and how they share it with others.

Over this period of engagement, participant groups took part in parallel learning of hydrology-focused scientific content and science communication principles, applying both to the creation of communication products, and synthesizing new knowledge and tools to engage effectively with peers and public audiences. Participants across this collection of programs created a wide range of science communication products, including hands-on activities, videos, games, audio products, and digital tools. Together, these methods and outcomes supported participants in communicating complex water and climate topics in accessible and meaningful ways.

This presentation will highlight educational approaches refined over a decade of programming, reaching over 10,000 in-person participants and a similarly sized audience through digital tools and lessons. Evaluation metrics collected across program iterations indicate consistent gains in self-reported knowledge and suggest positive participant experiences. It will also share core elements of the instructional framework and key lessons learned from a decade of communication and outreach, including observed impacts and practical insights for designing hands-on science communication experiences. By providing structured opportunities to both learn and practice science communication, these programs support participants in understanding how scientific knowledge is developed and communicated, with the broader goal of building trust in scientists and the scientific process.

How to cite: Gallagher, L., Pinchinat, J., Soriano, M., and Maxwell, R.: Learning, creating, and sharing: A science communication framework for water and climate education, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15455, https://doi.org/10.5194/egusphere-egu26-15455, 2026.

Recent advancements in AI technology have paved the way for the creation of sophisticated, educational avatars. These avatars are human-like in their interactions; they can listen to spoken input, generate appropriate responses, and communicate their answers through synthetic speech.  While AI-generated avatars are becoming more common for a variety of purposes in commercial sectors, they are rarely used in scientific fields. 

This technology represents a unique opportunity to reduce some of the roadblocks which can prevent students from pursing climate science as a career.  1) Many students, especially those from smaller communities, have never personally met a scientist, 2) they do not perceive climate science as a viable career path, and 3) students may not have been exposed to scientists who come from similar cultural backgrounds as themselves.  This project helps to address these challenges by bringing climate scientists directly into schools and communities, allowing students to have one-on-one conversations with scientists who can answer their questions and talk about science-related careers. AI avatars also enable students to engage with climate scientists who reflect their own appearances and cultural backgrounds, fostering a sense of relatability and inclusion.

Our team is creating AI-driven Virtual Climate Scientists who are trained to interact in real-time with both students and the general public.  These AI avatars are able to answer questions about their careers, current research in their field, and educational pathways that an interested student could consider. Each AI avatar represents a different field of climate science, and each has a different personal background, representing a wide range of cultures, educational backgrounds, life experiences, and personal stories.

We will present the current status of the project development, initial testing results from the beta-versions of the avatars, and lessons learned in the creation of each individual Virtual Climate Scientist.

How to cite: Brevik, C., Jayasekera, T., and Merriman, T.: Creating AI-driven Virtual Climate Scientists to introduce both students and the general public to climate science careers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15954, https://doi.org/10.5194/egusphere-egu26-15954, 2026.

In many parts of the world, fire is a key and natural disturbance on the landscape. However, they can have devastating environmental and economic consequences when they burn into urban interfaces, and when they burn at intensities and frequencies outside the adaptive capacity of native flora and fauna. In the modern era, vestiges of colonial fire management paradigms based on emergency response and fire suppression, and now coupled with the effects of climate change, have resulted in fires burning at unprecedented frequencies, sizes, and intensities, damaging ecosystems, livelihoods, and human populations. These effects highlight the need for a new fire management paradigm - one that integrates not just response and suppression, but also relevant sociocultural and environmental aspects.

Here, I present a range of outreach activities I have delivered across a range of audiences at science festivals in Europe and the UK, informed in part by findings from a survey carried out through the FIRE-ADAPT consortium, an EU funded project studying Integrated Fire Management (IFM). In the survey, participants were asked what they considered the most important actions for effective fire management. The most prevalent response was Public Outreach and Participation, highlighting the importance of targeting educational outreach, science communication, and public engagement in the development of fire management policy. The outreach activities I present here address two of the key messages respondents highlighted: 1) that fire is a natural, inevitable, and important part of fire-adapted landscapes, and 2) humans are a part of that landscape, and dispelling the nature-culture divide is essential for taking ownership of their participation in landscape management. I will discuss my motivations for engaging in these outreach activities, and how I see the key messages fit into broader fire management policies.

How to cite: Hsu, A.: Spreading like a Wildfire: The Importance of Education and Outreach in Fire Management, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16109, https://doi.org/10.5194/egusphere-egu26-16109, 2026.

In Saitama Museum of Rivers, workshops and exhibitions on soil have been organized for more than 10 years and we will share the experience in this presentation.

To recognize and stimulate curiosity towards soil, touching or observing soil and making participants feel the soil is effective. Long-run workshops carried out for the museum visitors who are not familiar with soil are, 1. making shining soil balls with clayey soil, 2. dying cloths with fluvial and volcanic soil, 3. stepping on soil of fluvial (paddy) and volcanic (upland farm) soil, 4. painting with soil of different color, 5. observing soil animals and others. All workshops include touching and/or observing soil. Main participant is primary school students and below with their parents. Questionnaire was taken for 2 hours workshops 1 and 2, and both showed high level of satisfaction. Free statement of the questionnaire were as follows, “Surprised that fine soil becomes so hard (1)”, “Could understand well about soil (1, 2)”, “Feels good with shiny surface (1)”, “Very much absorbed in the work (1, 2)”, “Surprised with the color difference of the two soils (2)”, “It was fun to knead the soil (2)”. From these answers, it can be said that participants enjoyed working on soil while learning about soil. It seems good that participants could bring what they made back home, too. From the experience of different workshops, it is important to talk casually about soil during the workshop (while participants are working on the today’s menu) not only to the young participants, but to their parents. Not the formal, lecture type but casual and relaxed talk stimulates curiosity to soil, which may lead to next question. As for exhibition, Soil Monolith Exhibition (2012), What is Soil (touring exhibition, 2015), Soil Watching (2023) were organized. “What is Soil” toured 13 different places, 7 of which content was fully exhibited and others partly, and number of total visitors was 50,757. Age of visitors is wide, and it was tried that contents would not be too technical yet keeping necessary information. Effort was made on hands-on and real material (e.g. monoliths) exhibits. From the questionnaire, visitors were satisfied because “could get to know about soil which is close to us but not familiar with”, “could actually see the real soil and touch the exhibits”, and not satisfied because “too technical and too many letters” (free statements). Contribution of soil monoliths to raise interest toward soil seemed high. Guide tours were arranged several times and they were popular, so face to face guide tour has great demand. Overall, satisfaction level was high and effective on people to get to know soil, with a room for better achievement.

How to cite: Mori, K. and Kosaki, T.: Appealing to the senses, long-run workshops and exhibitions on soil for museum visitors, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16330, https://doi.org/10.5194/egusphere-egu26-16330, 2026.

EGU26-16408 | Posters on site | EOS1.1

Public perceptions of cross-cascading climate change impacts: evidence from Bucharest, Romania 

Gabriela Ioana-Toroimac, Dana Maria Constantin (Oprea), Adrian Amadeus Tișcovschi, and Andreea Raluca Niculescu

The aim of the study was to identify cross-cascading impacts of climate change as perceived by the general public, in order to further develop strategies for education and awareness. The study employed an open-ended survey conducted in the city of Bucharest, located in southern Romania. Respondents were asked to provide examples of climate change impacts across different categories (environment, society, and economics).

The respondents identified a wide variety of environmental consequences, the most frequently mentioned being the increased frequency and/or magnitude of meteorological, climatic, and hydrological hazards. Drought ranked highest, being identified by 48% of all respondents. Public health emerged as the most important societal concern related to climate change (mentioned by 39% of respondents), with particular emphasis on the fatal effects of heat waves (designated by 10% of respondents). From an economic perspective, losses in agriculture were considered the most significant consequence of climate change by 59% of respondents.

In addition to these general findings, several specific perceptions emerged. 17% of respondents considered rising prices to be a consequence of climate change; in the context of water scarcity, they anticipated higher costs for irrigation, hydropower generation, fluvial transportation, and new methods to reduce water pollution, ultimately leading to higher prices of final products. This was followed by concerns regarding a decline in living standards. Furthermore, 20% of respondents indicated that industry and services are changing their structure in response to green requirements, while outdoor labor conditions are increasingly influenced by extreme weather, leading to labor market changes aimed at adapting to these new conditions.

The responses demonstrated a good understanding of the natural phenomena and processes occurring in southern Romania in recent years. They also revealed concerns regarding the future evolution of the economy. Overall, respondents showed a clear awareness of the cross-cascading impacts of climate change. However, climate change cannot be dissociated from other factors influencing social life and economic development; therefore, respondents’ perceptions are likely shaped by a multitude of contributing elements.

In a proactive approach, new curricula and academic study programs should be developed to address extreme weather, water scarcity, and the evolving labor market in southern Romania, in order to support career integration and ensure a sense of financial security.

How to cite: Ioana-Toroimac, G., Constantin (Oprea), D. M., Tișcovschi, A. A., and Niculescu, A. R.: Public perceptions of cross-cascading climate change impacts: evidence from Bucharest, Romania, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16408, https://doi.org/10.5194/egusphere-egu26-16408, 2026.

EGU26-17919 | Posters on site | EOS1.1

Analysis of Weather Broadcasting in Public Media: A Case Study of MTVA News and Weather Reports 

Csilla Molnár, Csilla Ilyés-Vincze, Ádám Leelőssy, and Zsuzsanna Soósné Dezső

The integration of meteorological information into public media is vital to promote public awareness and engagement. This study investigates the audience performance of the Hungarian Public Media (MTVA- Media Service Support and Asset Management Fund) weather reports and news broadcasts during 2023 and 2024. As extreme weather events and climate-retated issues increasingly shape daily life, the need for reliable and timely meteorological information has become more pronounced. This research examines how M1 channel’s weather reports influence viewer engagement, particularly in relation to broader television consumption habits and major socio-political events.  Using Nielsen Audience Measurement data, we analysed 13,758 weather reports, representing an average of 18-20 broadcasts per day. In the two-year period, these programmes accounted for 656 hours of airtime. The broadcasts reached more than 5.1 million viewers, covering 60.5% of the television audience aged four and above, with viewers watching an average of 78 weather reports annually.

Viewing patterns show clear peaks during early morning, midday, and evening news periods, closely linked to daily routines. Demographic analysis revealed that urban residents, particularly in Budapest, exhibit higher engagement rates compared to rural areas, reflecting global trends observed in studies such as those by the Pew Research Center and Nielsen. Additionally, older audiences (aged 60 and above) demonstrated the most consistent viewership, while the younger population (18-29 years of age) showed a preference for digital platforms over traditional television.

Using detailed audience data, the study explores how weather forecasts attract and retain viewers, highlighting factors such as broadcast timing, content organisation, and the placement of meteorological updates into news program.

Overall, the findings confirm that television remains a relevant and effective channel for meteorological communication, particularly among older and urban audiences. At the same time, the results emphasise the importance of strategically incorporating digital media in order to reach younger viewers more effectively. These insights contribute to ongoing discussions about optimising weather communication in the digital era and offer practical implications for public service broadcasters internationally.

How to cite: Molnár, C., Ilyés-Vincze, C., Leelőssy, Á., and Soósné Dezső, Z.: Analysis of Weather Broadcasting in Public Media: A Case Study of MTVA News and Weather Reports, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17919, https://doi.org/10.5194/egusphere-egu26-17919, 2026.

EGU26-18054 | Orals | EOS1.1

Communication within the UK flood hydrology community: bridging the gaps between science and practice  

Linda Speight, Emma Ford, Anita Asadullah, Louise Slater, Sally Brown, Helen Harfoot, Owain Sheppard, Chris Skinner, Clare Waller, and Thomas Willis

Flood hydrology sits at the interface of science, public protection, infrastructure planning, and regulation. It is a broad and interdisciplinary field; in a recent UK survey of users of hydrology only 45 % self-identified as a hydrologist. To ensure society is prepared for increasing hydrological risks, effective communication within this diverse community is essential. Without clear pathways for translation pathway between policy priorities, emerging research and operational needs, critical planning and policy decisions risk being made on outdated assumptions. However, operational decisions are not always able to draw upon the latest research into process understanding or modelling approaches due to multiple barriers. These barriers include uneven access to data and tools, capacity constraints, differences in incentives across sectors and the limited time for relationship building and knowledge translation across different expertise

Here, we present insights from around 60 participants at a “science into practice” workshop hosted at the British Hydrological Society Symposium (University of Oxford, September 2024). The workshop was designed as a sector-spanning exercise between researchers, consultants, regulators, and practioners working on flood hydrology across the UK. Across sectors, participants converged on six priority themes: (1) working together, (2) funding and responsibilities, (3) skills and training, (4) data, (5) methods, and (6) accreditation and usability. We reflect on how these themes provided insights into the challenges and opportunities for science communication, knowledge translation and collaboration, and why such activities are often undervalued despite their critical role for improving flood-risk decisions. We conclude with practical recommendations for improving “science into practice” pathways in flood hydrology with more inclusive cross-sector communication aligned with the goals of the co-developed 25-year UK Flood Hydrology Roadmap. These lessons learned are transferable to other areas of environmental risk where effective communication and collaboration are crucial for delivering societal and environmental benefits.  

How to cite: Speight, L., Ford, E., Asadullah, A., Slater, L., Brown, S., Harfoot, H., Sheppard, O., Skinner, C., Waller, C., and Willis, T.: Communication within the UK flood hydrology community: bridging the gaps between science and practice , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18054, https://doi.org/10.5194/egusphere-egu26-18054, 2026.

EGU26-20402 | Posters on site | EOS1.1

Perception of risk associated with tropical days in urban environments and implications for public health: A case study of Bucharest, Romania 

Dana Maria Constantin (Oprea), Gabriela Ioana-Toroimac, Elena Grigore, Adrian Amadeus Tișcovschi, Raul Gabriel Ilea, and Mihai Andrei Nițu

In most mid- and high-latitude regions, a decrease in the frequency of very low temperatures and an increase in the frequency of high temperatures have been observed as a consequence of ongoing global warming. Tropical days, defined as days with a maximum air temperature of at least 30°C, represent a key climatic indicator for assessing the impact of heat excess on the urban environment. The increasing frequency of these days in recent decades, amplified by the urban heat island effect, accentuates the thermal discomfort and the vulnerability of urban population.

The perception of risk associated with the increasing frequency of tropical days is influenced by the mode of institutional communication and by the availability of clear and credible early warning systems. The aim of this study is to quantify the level of information and awareness among the population of the Bucharest metropolitan area, the capital of Romania, regarding how the human body perceives and reacts to high air temperatures. Cities of Bucharest’s size can modify the air temperature, increasing it by approximately 5–6°C above the temperature of the surrounding area. The analysis was based on a questionnaire containing semi-open questions with multiple response options, applied individually and directly, to a sample of 267 participants. 44% of respondents reported feeling vulnerable to daily air temperature equal to or exceeding 30°C, 40% answered sometimes, in certain situations, and the rest that they are not vulnerable to such air temperature. Respondents associate, in decreasing order of the number of answers, excess heat with dehydration, fatigue and insomnia, irritability, respiratory problems, and muscle cramps and aches. As measures to improve living conditions during periods with tropical days, participants consider the need for more urban green spaces, greater environmental responsibility at both individual and collective levels (through systematic ecological and climate education), and the establishment of additional hydration and first aid points.

Integrating public perception into urban planning and public health policies is essential for reducing the risk associated with tropical days in cities and adapting to climate change, because thermal stress is not an isolated phenomenon but one that disproportionately affects the elderly, children, individuals with chronic illnesses, and low-income communities.

How to cite: Constantin (Oprea), D. M., Ioana-Toroimac, G., Grigore, E., Tișcovschi, A. A., Ilea, R. G., and Nițu, M. A.: Perception of risk associated with tropical days in urban environments and implications for public health: A case study of Bucharest, Romania, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20402, https://doi.org/10.5194/egusphere-egu26-20402, 2026.

EGU26-21016 | ECS | Orals | EOS1.1

Community organising and engaging young people with climate change research and policies 

Emma Hanson, Carl Stevenson, YouCAP members, Richard Campbell, Saidul Haque Saeed, and Sarah Greene

The inclusion of young people in climate change and palaeoclimate research has never been more important. There is a general uncertainty for our long-term future that is felt more within the young people within society, with climate anxiety a source of concern. Communication around climate change and palaeoclimate research to the general public is often in the form of education and traditional public engagements, such as social media, blogs and the press. 

Through work with Citizens UK, a diverse people-powered alliance of civil society institutions, we are working with a group of young people (aged 14-18) from a mixture of schools and city centre youth clubs based in deprived areas to create YouCAP, a youth climate advisory panel in the city of Birmingham. This work is linked to a larger NERC-funded project (C-FORCE) that is focusing on climate change in the past. We are training young people in broad-based community organising techniques, empowering them to speak to those in positions of power, like local councillors and leaders, and to conduct a local listening campaign about policy related to climate change. The first cohort of YouCAP participants found a general apathy for climate change issues in their communities, with many people naming personal issues such as the cost of living crisis or housing problems as higher priorities. The young people went on to create a podcast exchanging perspectives with those in power, with guests including a local councillor involved in city wide sustainability efforts, a scientist from the C-FORCE project, and a PhD student researching critical metals for the energy transition. Already YouCAP played a critical role in making climate change a national priority for Citizens UK and  leveraged the podcast recording with the local councillor to extract a promise of organising a youth climate assembly about local climate policy in the near future.

This work is ongoing, with continuous recruitment of new members of YouCAP, as well as the development of relationships with other key partners. Our final aim is to enact change at a local level with the work we have been doing with the young people through discussions around climate-related policies with local government leaders. By conducting this community engagement within the larger sphere of an international multi-disciplinary science project, a greater understanding of how the project outputs are absorbed by communities will be gained and trusting relationships will be formed with local communities, which is needed to convey the issues surrounding climate change to the public.

How to cite: Hanson, E., Stevenson, C., members, Y., Campbell, R., Haque Saeed, S., and Greene, S.: Community organising and engaging young people with climate change research and policies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21016, https://doi.org/10.5194/egusphere-egu26-21016, 2026.

EGU26-21176 | Orals | EOS1.1

From Knowledge Production to Societal Relevance in Earth Sciences 

Rosa Rodríguez Gasén and María Arista-Romero

Clearly, communication, dissemination and outreach play an increasingly important role in the social impact of research. Beyond performing solid and high-quality scientific knowledge, research centres are expected and required to ensure that the results obtained are accessible, useful, meaningful, and relevant to a wide range of publics and audiences.

This talk aims to showcase the communication, dissemination, and outreach activities implemented by the Earth Sciences Department at the Barcelona Supercomputing Center-Centro Nacional de Supercomputación (BS-CNS). The actions carried out in the field of communication and dissemination of Earth Sciences will be presented, and the lessons learnt and the challenges ahead for fostering the exchange of knowledge among various stakeholders, including (multidisciplinary) research teams, communication and dissemination professionals, and stakeholders, will be discussed.

The coordination of communication, dissemination and knowledge exchange activities within the framework of various research projects, which often pursue different objectives and have varying paces, will also be explained, as well as the role of teams dedicated to knowledge integration in building a bridge for dialogue with the user communities of the results obtained. The talk will explore how participatory approaches, co-creation processes, and different adaptive communication formats can contribute to reinforcing relevance, fostering mutual learning, and improving trust between researchers and stakeholders.

While sharing transferable lessons and questions that are still open, this overview aims to encourage ongoing discussions and debates about how research institutions, in our particular case in the scientific field of Earth Sciences, should move from simple ad hoc dissemination activities to more strategic, integrated, and impact-oriented communication and engagement practices in society.

How to cite: Rodríguez Gasén, R. and Arista-Romero, M.: From Knowledge Production to Societal Relevance in Earth Sciences, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21176, https://doi.org/10.5194/egusphere-egu26-21176, 2026.

EGU26-21456 | Orals | EOS1.1 | Highlight

Expanding the Space of Climate Agency: From Individual Decisions to System Dynamics 

Elena Claire Ricci, Giulia Tasquier, Francesca Pongiglione, and Sonia Morandi

Young people show a growing willingness to contribute to climate change mitigation, yet empirical evidence consistently highlights the persistence of misconceptions, fragmented knowledge, and difficulties in translating intentions into effective action. This lack of orientation is not surprising given the complexity of the socio‑ecological processes at stake. It is therefore crucial to develop educational tools to support individuals in critically engaging with these challenges, developing the ability to make informed decisions and take effective action. Supporting orientation toward agency in such contexts requires educational strategies capable of making systemic dynamics visible, explorable, and grounded in real-world data. This contribution is developed within the ENCOMPASS project, a multidisciplinary research initiative integrating perspectives from philosophy, economics, and science education to investigate agency in the context of climate change. ENCOMPASS conceptualises agency through three complementary and integrated lenses: epistemic-driven, ethical-refelctive and systemic-pragmatic. For this contribution, we focus on the systemic–pragmatic dimension of agency, which expands the space of action by linking individual decision-making to system-level dynamics and collective consequences.

It is specifically focused on food practices, i.e., day-to-day ‘simple’ decisions that offer significant individual climate-change mitigation opportunities. In particular, we study two key behaviours: reducing meat consumption and reducing food waste, analysing perceptions, barriers, and drivers of adoption.

The research follows two phases: (i) an exploratory qualitative analysis with students from two Italian upper‑secondary schools through focus groups, which generated concept maps used to identify the most crucial issues and thus relevant variables; (ii) the design and administration of a structured survey to a representative sample of the Italian population (N=1400).

The survey investigated individual food-related choices and behaviours in real contexts with a strong focus on the motivations and the characteristics of the context in which they were taken. Moreover, through the use of validated scales we evaluate perceptions, concerns, values, knowledge, social and moral norms of respondents. These dimensions allow for a detailed analysis of how beliefs, cognitive factors, social influences, and socio-demographic characteristics affect individual adoption of more climate-friendly and sustainable food-practices. The outputs of the analysis of this data collection are used as the empirical base to calibrate a system-dynamics simulation-model identifying potential dynamics of behaviour adoption among individuals. This modelling can generate interactive scenarios showing the (aggregated) effects of changes to individual behaviours, which could potentially contribute to strengthen youth orientation toward sustainable food-choices.

The model enables the exploration of feedback mechanisms and scenario-based outcomes, illustrating how individual decisions may aggregate and evolve within a complex system over time. We argue that empirically grounded SD simulations can function as powerful educational tools, supporting learners in critically engaging with complex socio-ecological processes, exploring “what-if” scenarios, and understanding the systemic implications of everyday decisions. By bridging individual action, empirical data, and system-level modelling, this work contributes to expanding the space of climate agency in education and beyond.

The proposed modelling approach allows agency to be examined through the dynamic relations between individual decisions and system-level outcomes, offering a concrete way to analyse how possibilities for action are shaped, enabled, and constrained within complex socio-ecological systems.

How to cite: Ricci, E. C., Tasquier, G., Pongiglione, F., and Morandi, S.: Expanding the Space of Climate Agency: From Individual Decisions to System Dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21456, https://doi.org/10.5194/egusphere-egu26-21456, 2026.

EGU26-21462 | ECS | Posters on site | EOS1.1

Using Environmental Observatory Data from the Navarino Environmental Observatory (NEO) to Advance Climate Change Education in the Mediterranean 

Georgios Maneas, Christos Pantazis, and Martina Hättestrand

Environmental observatories provide powerful real-world contexts for advancing climate change education and fostering engagement with Earth system science. The Navarino Environmental Observatory (NEO), located in southwestern Greece, integrates long-term environmental monitoring with interdisciplinary research, generating high-resolution datasets on atmospheric conditions, ecosystem dynamics, soil and hydrological processes, and biodiversity change in a Mediterranean climate hotspot. By linking empirical observations to education and outreach activities, NEO supports learning experiences that connect scientific evidence to place-based climate impacts and societal challenges.

This contribution presents how NEO observational data are embedded in participatory education initiatives to enhance climate literacy, critical thinking, and data competencies across diverse learner groups. Drawing on examples from international field courses, summer schools, living lab activities, and community workshops, we show how students and stakeholders engage directly with real environmental datasets to interpret trends, explore uncertainty, and understand feedbacks between climate, ecosystems, and land management. Particular attention is given to how data-driven learning influences climate perceptions, supports interdisciplinary understanding, and encourages informed dialogue between scientists and society.

Our experience demonstrates that combining long-term environmental observations with experiential and participatory educational approaches strengthens climate change education, promotes trust in scientific evidence, and supports the development of actionable knowledge for climate adaptation and sustainability.

How to cite: Maneas, G., Pantazis, C., and Hättestrand, M.: Using Environmental Observatory Data from the Navarino Environmental Observatory (NEO) to Advance Climate Change Education in the Mediterranean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21462, https://doi.org/10.5194/egusphere-egu26-21462, 2026.

The communication of paleontological heritage to non-specialist audiences presents unique challenges: fossils are fragmentary, ancient environments are invisible, and the scientific reasoning connecting evidence to reconstruction is often opaque. This contribution examines how generative artificial intelligence and three-dimensional digital technologies are transforming science communication practice in paleontology while proposing an epistemological framework to ensure scientific integrity in public engagement.

We present a four-paradigm classification distinguishing: (1) Empirical methods (photogrammetry, structured-light scanning, LiDAR) that produce metrically accurate digital surrogates of physical specimens; (2) Neural Scene Representation (Neural Radiance Fields, 3D Gaussian Splatting) that reconstruct scenes from sparse image sets through learned interpolation; (3) Generative AI (diffusion models, large language models, image-to-video synthesis) that create novel content based on pattern recognition rather than direct observation; and (4) Hybrid approaches that combine two or more methodologies. This framework addresses a fundamental question for science communicators: whether a given digital output constitutes a record, a representation, or a hypothesis—a distinction critical for maintaining public trust.

We demonstrate applications ranging from constraint-based paleoartistic reconstruction to AI-generated video synthesis for museum exhibitions and educational programs using real-world workflows created at Centro Ciência Viva de Lagos, Portugal, as part of the PaNReD (ALG-07-527-FSE-000044) and SciTour (ALG-01-0145-FEDER-072585) projects. A key case study involves the digital reconstruction workflow for Cariocecus bocagei, a new hadrosauroid from the Lower Cretaceous of Portugal, illustrating the complete pipeline from photogrammetric capture of fossil specimens through AI-assisted life reconstruction and video generation. This process illustrates how empirical 3D models function as anatomical constraints for generative AI, guaranteeing that paleoart remains connected to physical evidence while simultaneously achieving the visual impact required for effective public engagement. We critically examine the phenomenon of “hallucinated heritage”—the risk that visually convincing AI outputs may inadvertently disseminate subtle biases or fabrications to public audiences who lack the expertise to distinguish evidence-based reconstruction from algorithmic speculation.

The most challenging obstacle we have faced is the preservation of the distinction between what is known from fossil evidence and what is inferred or imagined, especially when AI-generated imagery attains a photorealistic quality that may imply false certainty. Our approach addresses this through explicit labeling of epistemological status, transparent documentation of AI prompts and constraints, and educational materials that use the reconstruction process itself as a teaching tool about scientific reasoning.

We argue that these technologies do not diminish the role of the scientist-communicator but rather transform it from “guardian of the rock” to “authenticator of reality.” The emotional connection fostered by immersive 3D environments and lifelike paleoart reconstructions can enhance public engagement with deep time, provided that communication strategies explicitly address the epistemological status of digital outputs. This session contribution shares lessons learned from five years of integrating digital technologies into science centre programming, offering a framework for practitioners seeking to harness AI's communicative power while preserving scientific integrity.

How to cite: Azevedo Rodrigues, L.: Generative AI and 3D Digital Technologies for Paleontological Heritage Communication: An Epistemological Framework and Practical Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21526, https://doi.org/10.5194/egusphere-egu26-21526, 2026.

EGU26-21602 | Posters on site | EOS1.1

Acknowledging different levels of audience engagement in science in research outreach strategies 

Timothy D. James, Guðfinna Aðalgeirsdóttir, Christine S. Hvidberg, and Eliza Cook and the ICELINK Team

The outreach strategies of research projects often focus on ambitious objectives such as improving the knowledge base for stakeholders, promoting uptake of informed strategies and societal transitions, increasing awareness of research, etc. However, objectives like these take for granted that target audiences are engaged in science and trustful of expertise when we know that there is a growing population throughout society who are neither. The growing mistrust of science and experts is, at least in part, a failure of the science community to reach and engage with a significant sector of society.  In an attempt to address this deficiency in our own work, the ICELINK project aims to tailor key messages to identified target audiences that acknowledge these differing levels of engagement and trust.  While recognizing target audiences, including local stakeholders, policymakers, and the general public, we also recognize that within these audiences we will find individuals and groups who are:

  • highly engaged (e.g., those who would, for example, eagerly attend a public science event);
  • marginally engaged (e.g., those who would attend a public science event if it were convenient or brought to them, but might not actively seek one out); and
  • unengaged (e.g., those who would not attend a public science event without some external motivator).

While scientists tend to excel at engaging with members of the public who are highly and marginally engaged in science, those in the third category are at high risk of being overlooked. With this in mind, in addition to sharing ICELINK’s science objectives, results, and outputs in innovative and creative ways, we also intend to help rebuild trust in science by sharing messages of greater relevance to less engaged audiences. For example, when communicating about climate change, we aim to use more positive messaging of hope and empowerment through personal action, an approach that is thought to increase an audience’s receptiveness compared to focusing solely on the consequences of climate change and inaction. We can also help make scientists (and experts generally) more relatable through personal perspective storytelling, and we will use “lightening experiences” (a.k.a. the “wow factor”) to help audiences appreciate difficult-to-grasp concepts (like vast spatial and temporal scales) and to remind people about the power and possibilities of science.

Scientists need to be better at reaching more diverse members of the general public. When planning our outreach strategies, if we can adjust our pathways to engagement, messaging, and expectations to be relevant to the full engagement/trust spectrum, perhaps we can have more of an impact on all audiences.

How to cite: James, T. D., Aðalgeirsdóttir, G., Hvidberg, C. S., and Cook, E. and the ICELINK Team: Acknowledging different levels of audience engagement in science in research outreach strategies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21602, https://doi.org/10.5194/egusphere-egu26-21602, 2026.

Social media has become a key bridge between the scientific community and the broader public. Early Career Researchers (ECRs) in Latin America have increasingly embraced digital platforms to engage non-specialist audiences with geosciences content, especially during the COVID-19 pandemic. One such initiative is Divulgación Terróloga, a non-profit, self-funded science communication project launched on June 11, 2019, by Mexican ECRs. The project aims to communicate Earth system processes clearly and accurately in Spanish through Facebook and Instagram. Our content covers all Earth spheres topics and features regular posts that promote the visibility of geosciences and the scientific work of mainly ECRs. The section "Miércoles de Jóvenes Investigadores" (Young Researchers Wednesday) highlights the research of students and early-career scientists, while the section "Geocientíficos en Acción" (Geoscientists in Action) focuses on geoscientists working beyond academia. We also conduct interviews with established researchers to highlight diverse career paths. In this presentation, we share the scope, challenges, and impacts of running Divulgación Terróloga. By April 23, 2025, we have published ~360 posts, reached ~2200 people per post on average, and grown a following of over 5300, with our most popular post reaching nearly 60,000 views. The audience is gender-balanced (49% women, 51% men) and spans Latin America, the U.S., and Europe. Our posts have been translated automatically into English, French, and German. This talk aims to highlight the power of social media in promoting geosciences education, increasing the visibility of ECRs, and building international scientific networks and bridges with society through outreach.

How to cite: Martinez-Abarca, R.: A guide to outreach geosciences on social media: the case of Divulgación Terróloga, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21614, https://doi.org/10.5194/egusphere-egu26-21614, 2026.

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