Presentation type:
GI – Geosciences Instrumentation & Data Systems

With the rapid development of artificial intelligence (AI), energy consumption and carbon emissions from high-demand computing power have gradually attracted widespread attention in the environmental field. Existing research largely focuses on data centers, which are the infrastructure that directly generates AI-related carbon emissions. However, the users who truly drive computing power demand have long been neglected. A major reason is the difficulty in tracking and accurately locating users, so that AI-related carbon emissions from users’ perspective have lacked systematic identification and discussion so far. It is worth noting that with the wide application of AI, the primary source of carbon emissions has shifted from model training to large-scale and multi-domain usage. This means that understanding the spatial distribution pattern of AI users is crucial to explore demand-side emission reduction in AI, especially during periods of bottlenecks in production-side emission reduction, such as the slow green transformation of the electricity energy mix. Demand-side management can, to some extent, contribute to mitigating AI-related carbon emissions. In this study, we aim to display the spatial distribution of AI users within the city and assess whether variations in usage across different wards may lead to potential spatial inequalities in AI-related carbon emissions. Taking London as a case study, we utilize regional AI penetration rates and AI user profiles to spatially decompose urban AI users at a more granular scale, quantifying the corresponding AI-related carbon emissions and comparing the proportion of AI-related carbon emissions in residents' carbon footprints and potential inequalities. We expect to find spatial clustering of AI-related carbon emissions and a positive correlation with the distribution of educational resources and wealth. Our study may provide an empirical basis for understanding the new environmental inequalities brought about by AI development and offers key references for future green digital governance on the demand side.

How to cite: Yin, Y., Chu, Y., and Chen, Y.: Mapping AI Users and Potential Inequality Pattern: A Spatial Downscaling Study in London, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-895, https://doi.org/10.5194/egusphere-egu26-895, 2026.

Gridded population datasets play a pivotal role in a wide range of contemporary research and development, such as the distribution of aid, public health campaigns, as well as disaster risk management. However, the selection of the appropriate existing population dataset remains a non-trivial task, resulting in many practitioners choosing based on convenience or familiarity, rather than explicit use-case suitability.

In our contribution we present a user-requirement driven review of major gridded population datasets, in particular reviewing the wide array of the WorldPop suite, including their bespoke datasets, LandScan (HD), Kontur, Facebook HRSL, GPW, and GHS-Pop. We first consolidate key requirements of users in applied human-environment research and policy, based both on a literature review as well as key-informant-interviews of practitioners in the Humanitarian sector. Our synthesis reveals barriers to informed dataset choice, including scattered and inadequate documentation, limited uncertainty quantification and communication, and a lack of explicit suitability statements.

We then systematically evaluate, based on Riedler et al., 2025 (under review), how current existing datasets perform with respect to spatial granularity, temporal consistency, sensitivity to input data, the influence of settlement type on accuracy, and transparency of the product.

Based on the combination of both findings, we derive a set of generalised guiding questions for practitioners, as well as a decision tool for use-case specific dataset choice. We, furthermore, illustrate the effects of different dataset choices on down-stream applications and their potential impact on decision-making, as well as discussing alternative methods to establish population estimates and their suitability for studies and policies.

By shifting the perspective from dataset-centric descriptions to user-centred logic our review provides a foundation for operational decision-support and better understanding of gridded population products for domain agnostic users.

How to cite: Klaussner, E. S.: Towards Informed Use of Gridded Population Data: A User-Driven Selection Framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1294, https://doi.org/10.5194/egusphere-egu26-1294, 2026.

EGU26-3779 | ECS | Posters on site | ITS1.14/GI1

Geospatial Assessment of Sustainable Ecotourism Potential in Naryn, Kyrgyz Republic 

Koisun Darylkan kyzy, Lukas Lehnert, and Kobogon Atyshov

The present study aims to identify potential areas for the development of sustainable ecotourism in the Naryn Region of the Kyrgyz Republic using geographic information systems (GIS) and weighted overlay methods based on Earth remote sensing data. Ecotourism is one of the most dynamically developing and economically promising sectors oriented toward sustainable territorial development. The Naryn Region possesses significant potential for ecotourism development due to its mountainous terrain, unique natural landscapes, rich biodiversity, and cultural heritage. The weighted overlay method is an effective and visually intuitive tool for comparing multiple thematic layers, whose values are determined based on natural, environmental, and socio-economic factors. The study utilizes open-access geospatial data, including satellite imagery and digital elevation models. Data processing and analysis are carried out using ArcGIS software and specialized remote sensing applications. Seven thematic layers are employed in the analysis: elevation above sea level, land use and land cover, proximity to water bodies, transportation accessibility, population density, proximity to protected areas, and natural and cultural heritage sites. Based on the physical-geographical and socio-cultural characteristics of the Naryn Region, weighting coefficients are assigned to each thematic layer, followed by an integrated suitability analysis. As a result, an ecotourism suitability map is generated and classified into five categories from very high to very low suitability. The results demonstrate the potential of specific areas within the Naryn Region for sustainable ecotourism development while simultaneously accounting for environmental protection constraints.

How to cite: Darylkan kyzy, K., Lehnert, L., and Atyshov, K.: Geospatial Assessment of Sustainable Ecotourism Potential in Naryn, Kyrgyz Republic, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3779, https://doi.org/10.5194/egusphere-egu26-3779, 2026.

EGU26-7631 | ECS | Posters on site | ITS1.14/GI1

Do disasters speak louder than hazard exposure? Tourism policy and ecosystem protection in coastal destinations 

Vilane Goncalves Sales and Marie Fujitani
Tourism in tropical coastal regions depends fundamentally on healthy ecosystems, yet tourism policies often fail to acknowledge this social-ecological interdependence. While environmental and climate adaptation policies may address ecosystem protection, the tourism sector frequently overlooks ecosystem safeguards in its own policy frameworks. This sectoral disconnect raises a critical question: what drives tourism policymakers to articulate protection for the ecosystems their sector relies upon? Do they respond proactively to known hazard risks, or does disaster experience prompt greater policy attention to ecosystem protection? We investigated this question by analyzing 415 tourism policy documents from 123 tropical coastal countries across a 25-year period (2000-2025). We developed a Tourism Ecosystem Protection Index (TEPI) using natural language processing to quantify policy articulation across five dimensions: ecosystem recognition, site management, infrastructure safeguards, environmental integration, and climate awareness. We combined this index with hazard exposure data from the INFORM Risk Index and realized disaster impacts from the EM-DAT database to test competing hypotheses about policy development.

Our cross-sectional analysis found no significant relationship between hazard exposure and tourism policy articulation of ecosystem protection. Countries facing severe cyclone and flood risks showed no greater policy attention to ecosystems than lower-risk destinations. Awareness of risk, it appears, does not translate into sectoral policy articulation. However, a different pattern emerged when examining countries that experienced major disasters. Using a quasi-experimental design comparing disaster-affected nations  to matched controls, we found that disaster experience was associated with greater policy articulation of ecosystem protection. This effect was concentrated in ecosystem recognition and environmental integration components, suggesting disasters may prompt reframing of tourism-environment relationships rather than merely technical adjustments. We note this represents changes in policy articulation, not demonstrated implementation.

Over our study period, the cross-sectional relationship between hazard exposure and policy articulation strengthened, with rolling correlations shifting from weakly negative to weakly positive. Three sensitivity analyses examining Zika virus, oil price shocks, and the Paris Agreement produced patterns consistent with a hazard-specific rather than general crisis or global governance mechanism, though these supplementary tests have limited statistical power. These findings carry provisional implications for climate adaptation in coastal social-ecological systems. Tourism policy may develop ecosystem protection articulation through reactive rather than anticipatory pathways. Disasters appear to prompt policy attention that general hazard awareness does not, though whether such articulation translates to implementation remains an open question requiring future research with outcome indicators.

How to cite: Goncalves Sales, V. and Fujitani, M.: Do disasters speak louder than hazard exposure? Tourism policy and ecosystem protection in coastal destinations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7631, https://doi.org/10.5194/egusphere-egu26-7631, 2026.

Whistler-Blackcomb is a premier ski resort in Canada, attracting approximately 2 million visitors annually and is about a two-hour drive from Vancouver, British Columbia. Whistler-Blackcomb has approximately 3,300 hectares of skiable terrain, a peak elevation of 2,240 meters, and a vertical drop of approximately 1,565 meters. Located at the ski resort are two weather stations: one at 659 meters (the resort Village) and a second at 1,835 meters (Roundhouse Lodge). These weather stations have been collecting daily data on air temperature, snowfall, rainfall, and ground snow depth since the 1970s. The Village weather station data record spans from 1977 to 2025. At this weather station, minimum temperatures, averaged for the winter season, are rising much faster than maximum temperatures (0.44 vs 0.10 °C per decade). Snowfall and rainfall show no noteworthy trends at the Village from 1977 to 2008. Measurements of these two variables were not made from 2009 to 2025. Ground snow depth appears to have declined significantly since 2009. The Roundhouse Lodge weather station data record spans from 1974 to 2025. At this location, average winter minimum temperatures are also rising faster than maximum temperatures (0.22 vs 0.11 °C per decade). No meaningful change in snowfall was observed at Roundhouse Lodge. However, winter rainfall has increased considerably since the early 2000s. Ground snow depth during the winter season shows no trend at the Roundhouse location. Finally, a stochastic weather generator, combined with an eight-member AR6 climate model ensemble (with an equilibrium climate sensitivity of 3.2 °C) and the emission scenarios SSP2-4.5 and SSP5-8.5, is employed to predict how daily minimum and maximum temperatures averaged over the winter season will change from 2030 to 2090.

How to cite: Pidwirny, M.: Changes in Temperature, Snowfall, Rainfall, and Ground Snow Depth Observed in Winter Daily Weather Station Data Collected at 659 and 1835 Meters from the 1970s to 2025 at Whistler-Blackcomb Ski Resort., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8452, https://doi.org/10.5194/egusphere-egu26-8452, 2026.

Urban and suburban forests provide major cultural ecosystem services, yet planning still often relies on destination-based indicators (e.g., nearest forest, simple distance buffers). These measures miss how real access is shaped by corridor continuity, available transport modes, and last-mile connections to entrances. As a result, they can misrepresent both visitation pressure and equity patterns across a metropolitan region.

We analyse forest recreation in the Vienna Metropolitan Area using representative Public Participation GIS (PPGIS) data (n = 3,121). We link anonymised home locations to reported forest destinations and entrances, derive origin–destination (OD) flows, and assess accessibility using both Euclidean distance and mode-specific network travel times for walking, cycling, public transport, and car. To move beyond a destination-only assessment, we apply density-based OD flow clustering (DBSCAN/HDBSCAN) to detect corridor-like patterns and compare clusters by travel time, mode share, and visitation frequency.

We identify six visitor groups (with sub-clusters in the two largest), differing in mobility profiles and spatial structure. We find a clear distance–decay relationship: each additional kilometre to the forest is associated with ~11% fewer annual visits. Importantly, distance alone does not explain use. Corridor structure matters. Multimodal “belts” around the city support access within feasible travel times, while other areas remain underused despite being geographically close, suggesting gaps in connectors and continuity rather than limited forest supply.

This corridor-based perspective complements destination-centric metrics and supports more actionable planning and mitigating environmental impacts. Strengthening gateways and last-mile links, protecting high-performing multimodal corridors, and targeting specific accessibility gaps can improve equity while limiting car dependence.

How to cite: Stefan, F.: Beyond distance: mapping multimodal forest recreation corridors in the Vienna metropolitan area using PPGIS and origin–destination flow clustering, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11718, https://doi.org/10.5194/egusphere-egu26-11718, 2026.

EGU26-15386 | Orals | ITS1.14/GI1

FuturePop - Constructing global gridded population maps at multiple scales for SSP scenarios  

Laurence Hawker, Maksym Bondarenko, Jason Hilton, Evgeny Noi, Natalia Tejedor Garavito, Rhorom Priyatikanto, Tom McKeen, Tomohiro Tanaka, and Andrew Tatem

Climate change significantly impacts health, environments, and socioeconomics, but these effects are not evenly distributed globally. Variations in the spatial distribution, age and sex structure, and rate of growth of human populations drive different vulnerabilities to climate change. Maps of future population scenarios are therefore essential for understanding, planning, and responding to these impacts now and long into the future. 

While efforts have been made to generate gridded future population maps, key gaps remain: a) consistency with historical datasets containing population (e.g., HYDE) for climate simulations; b) updates aligned with the latest SSP estimates; c) use of up-to-date data and methods; d) high-resolution outputs (100m) to support detailed climate impact studies; e) disaggregation by age/sex to assess specific vulnerabilities; and f) inclusion and communication of uncertainty. To address these, we launched the FuturePop project. 

Here we present the latest updates to FuturePop. FuturePop V0.2 (Bondarenko et al., 2025) produced 1km global maps for population count between 2025 to 2100 from the latest Shared Socio-economic Pathway (SSP) population estimates (SSP Database V3.2), with these maps now extended to 2300. In turn this FuturePop data has been harmonized with past (HYDE & GHS-Pop) and present (WorldPop) population data to contribute to CMIP7 forcing data (Paprotny et al., 2025), with extensions made until 2300. 

We present our initial maps for FuturePop V1.0. FuturePop V1.0 adds enhancements by explicitly incorporating SSP urbanisation rates and using SSP informed building volume estimates for spatial disaggregation. The latest work to create sub-national SSP population estimates and progress to create age/sex disaggregated maps will also be introduced.  

Lastly, we present initial maps from “FuturePop Japan.” These are informed by Japanese adaptations of the SSPs (Chen et al., 2020), which provide greater national nuance than the global SSPs. Japan is a particularly interesting case, as its population is ageing and declining. It also had a high building vacancy rate of 22% in 2015, projected to reach 66–78% by 2100 (Yoshikawa et al., 2025). Although Japan is extreme, understanding how to spatially disaggregate shrinking populations is critical, as nearly 60% of countries are projected to decline by 2100 under SSP Database V3.2. We focus on the Japan SSP1 scenario, which includes planned urban compaction through the government-led “compact plus network” initiative.  

  • Bondarenko, M., Tejedor Garavito, N., Priyatikanto, R., Zhang, W., Fang, W., Nosatiuk, B., & Tatem, A. (2025). Global 1-km population projections for 2025–2100 under SSP3.2 (v0.2). University of Southampton. https://doi.org/10.5258/SOTON/WP00849 
  • Paprotny, D., Hawker, L., Bondarenko, M., Hilton, J., Garavito, N. T., Noi, E., & Tatem, A. (2025). input4MIPs: CMIP7 PIK-CMIP-1-0-0. Oak Ridge National Laboratory. https://doi.org/10.25981/ESGF.input4MIPs.CMIP7/2583900  
  • Chen, H., Matsuhashi, K., Takahashi, K., Fujimori, S., Honjo, K., & Gomi, K. (2020). Adapting shared socioeconomic pathways for Japan. Sustainability Science, 15(3), 985–1000. https://doi.org/10.1007/s11625-019-00780-y  
  • Yoshikawa, S., Imamura, K., Takahashi, K., & Matsuhashi, K. (2025). Development of scenarios for climate impacts in Japan. In N. Mimura & S. Takewaka (Eds.), Climate Change Impacts and Adaptation in Japan (Springer). https://doi.org/10.1007/978-981-96-2436-2_36-2436-2_3 

How to cite: Hawker, L., Bondarenko, M., Hilton, J., Noi, E., Tejedor Garavito, N., Priyatikanto, R., McKeen, T., Tanaka, T., and Tatem, A.: FuturePop - Constructing global gridded population maps at multiple scales for SSP scenarios , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15386, https://doi.org/10.5194/egusphere-egu26-15386, 2026.

EGU26-16302 | Posters on site | ITS1.14/GI1

Application of a Gridded Population Dataset to the Projection of Cropland Potential under Workforce Constraints 

Nicklas Forsell, Hongtak Lee, and Hyungjun Kim

While ongoing climate change is projected to expand environmentally suitable cropland toward high-latitude regions, the practical utilization of this potential is increasingly shaped by socio-economic constraints. Previous studies have suggested that agricultural workforce availability, as a proxy for socio-economic transitions and interactions, acts as a bottleneck for cropland supply potential. In this study, we assess spatially explicit practical cropland supply potential by incorporating agricultural workforce constraints using gridded population datasets from WorldPop. A weighting map of agricultural workforce distribution was constructed based on national-level minimum distance thresholds between population pixels and cropland pixels, and was used to allocate agricultural labor spatially. Future cropland potential was then derived by applying land-to-labor ratios that represent technological advancement. Within this workflow, urbanization levels were reviewed by comparing WorldPop Global 1 and Global 2 datasets and population projection datasets, all classified based on DEGURBA definitions (EUROSTAT), with national urbanization statistics from the World Bank. In addition, agricultural workforce shares between rural and urban pixels were evaluated through comparison with ILO statistics. Our results indicate that agricultural workforce availability constrains the northward expansion of cultivable land. A southward retreat of workforce-available cropland potential is also projected in some regions, such as Central Asia, despite increasing environmental suitability. Beyond regional projections, this study further demonstrates an application channel through which high-resolution population datasets can be used to constrain and quantify human influences on the Earth system.

Acknowledgment: This research was supported by the National Research Foundation of Korea (NRF) grant funded by the Ministry of Science and ICT (RS-2021-NR055516, RS-2025-02312954).

How to cite: Forsell, N., Lee, H., and Kim, H.: Application of a Gridded Population Dataset to the Projection of Cropland Potential under Workforce Constraints, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16302, https://doi.org/10.5194/egusphere-egu26-16302, 2026.

EGU26-19312 | ECS | Orals | ITS1.14/GI1

From human mobility to urban service networks: a distance-based model for systemic risk assessment 

Marcello Arosio, Nicolò Fidelibus, and Michele Starnini

The construction of a network for assigning users to essential socio-economic services at the urban level provides a powerful framework to represent the web of functional connections that are exposed to natural hazards. Such a representation is particularly relevant for natural risk assessments, as it enables the analysis not only of direct damages to assets and services, but also of indirect and cascading impacts arising from service disruptions and user reallocation processes (e.g. during flood events). Building this type of network requires an understanding of decision-making factors, both individual and non-individual, which depend on multiple parameters, from economic to social. Despite this complexity, it is possible to reduce the modelling of these mechanisms to the analysis of a limited set of behavioural variables, such as the distance between the service and the user’s residence.

Based on millions of human movements, we highlight how to generate realistic flows of home–essential service users on an urban scale according to a distance-based universal law of service attractiveness. To do this, we incorporate the city road network into the distribution of populated buildings using demographic data, assigning an attractiveness value to the path to the service among all possible choices.

By showing how the universal law of service attractiveness depends on the size of the city, our study demonstrates that the larger the city under analysis, the more rapidly the attractiveness distribution of the service declines, and vice versa. Moreover, we highlight how service attractiveness is influenced by the type of essential service selected, distinguishing those for which people are most willing to travel long distances in order to benefit from them.

Our model, in addition to enabling the generation of a socio-economic network of assigned users to essential services—useful for various areas of research such as epidemiology and urban risk—bridges the gap between distance- and opportunity-based models of human mobility, characterising users’ decision-making mechanisms across multiple spatial scales and for different types of essential services through a distance-based universal law of service attractiveness.

How to cite: Arosio, M., Fidelibus, N., and Starnini, M.: From human mobility to urban service networks: a distance-based model for systemic risk assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19312, https://doi.org/10.5194/egusphere-egu26-19312, 2026.

EGU26-19353 | Posters on site | ITS1.14/GI1

A systematic review of the use of gridded population datasets in the assessment of climate-health risks 

Dorothea Woods, Jessica Esepey, and Amy Bonnie

The global climate crisis poses a growing and multifaceted threat to human health. Assessing and mitigating these climate-related health risks requires spatially explicit understanding of where populations are exposed and vulnerable to climate hazards. Advances in geospatial technologies and the increasing availability of satellite and remote sensing data have enabled the development of high-resolution global gridded population datasets, which have become critical infrastructure for climate-health research. These datasets support the analysis of population exposure and vulnerability across regions and scales, and are increasingly important for scenario-based assessments aligned with future climate and socioeconomic pathways.

This study systematically reviews academic literature published since 2015 to assess how gridded population data are being used in climate change and health research. Specifically, we examine who is using gridded population datasets, in which geographical regions, and for what types of climate-related health analyses. We assess the types of gridded population products used, including their spatial resolution and levels of demographic disaggregation, and how population data are integrated with climate and health information. Where reported, we also evaluate how study results are interpreted and applied to inform policy or decision-making.

The review of 222 academic peer-reviewed studies demonstrates that i) gridded population data have become foundational infrastructure for climate–health research, with a marked increase in publications since 2015; ii) applications span multiple health domains; iii) there is a substantial geographical imbalance; iv) gridded population data enable assessments of population exposure and vulnerability; v) use of age- and sex-disaggregated data is limited.

Overall, the review highlights gridded population data as a crucial bridge between climate science and public health action, emphasising the need for continued dataset development, interdisciplinary collaboration, and integration with future climate and socio-economic scenarios.

How to cite: Woods, D., Esepey, J., and Bonnie, A.: A systematic review of the use of gridded population datasets in the assessment of climate-health risks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19353, https://doi.org/10.5194/egusphere-egu26-19353, 2026.

EGU26-20185 | ECS | Orals | ITS1.14/GI1

The Role of Gridded Population Data in Shaping Future Exposure Estimates 

Heather Chamberlain, James Savage, and Laurence Hawker

The impact of climate change on human populations is already being felt around the world. Both its effects, and the human populations affected, are unevenly distributed, driving differential exposure and vulnerabilities. To better understand, plan for, and respond to climate change impacts, mapped estimates of population projected under future SSP (Shared Socioeconomic Pathway) scenarios have been developed.

With a growing number of SSP-consistent gridded population datasets being developed - over thirty to date - the comparability of these datasets needs to be understood. If these datasets are used in hazard exposure analyses or vulnerability assessments, the choice of gridded population dataset potentially has a considerable impact on the population estimated to be at risk. Research on the impact of dataset choice in such analyses has been very limited. In this work, we start to address these knowledge gaps. Firstly, we introduce results of a comparative review of existing gridded future population estimates. We explore how differences in: (i) SSP database versions, (ii) downscaling methods, and (iii) classification of built settlement and urban areas, translate into variability at the grid cell level. The results of our comparative analysis show that fundamental differences exist between the various SSP-consistent future gridded population datasets.

Secondly, we focus on the challenges that differences in gridded population dataset bring for downstream data users, with an example of assessing future population exposure to flood hazards in parts of China and Italy. Using flood extents, derived from a high-resolution hydrodynamic flood model, for four time points (2020, 2050, 2070 and 2100), we calculate an estimate of exposed population based on each gridded population dataset. Preliminary results show that flooding exposure estimates vary considerably depending on which gridded population dataset is used. Our results underscore the critical role that accurate future small area population estimates have in robust exposure and vulnerability analyses.

How to cite: Chamberlain, H., Savage, J., and Hawker, L.: The Role of Gridded Population Data in Shaping Future Exposure Estimates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20185, https://doi.org/10.5194/egusphere-egu26-20185, 2026.

EGU26-20475 | Orals | ITS1.14/GI1

Advances in producing and evaluating gridded population data at the European Commission’s Joint Research Centre 

Johannes Uhl, Marcello Schiavina, Cristian Pigaiani, Filipe Batista e Silva, Alfredo Alessandrini, Sergio Freire, Katarzyna Krasnodębska, Alessandra Carioli, Martino Pesaresi, Thomas Kemper, and Lewis Dijkstra

The European Commission’s Joint Research Centre (JRC) produces open and free gridded data on human settlements and population at the European and global level. These datasets provide robust sources for decision making, planning, disaster risk management and scientific research. In this talk, we will provide an overview of recent developments and advances with this regard. Specifically, we will highlight ongoing work, novel datasets and underlying methods, including global, gridded future projections (GHS-WUP-POP; 1-km population estimates from 1980 to 2100), historical gridded population data for Europe since the 1960s using spatially-explicit backcasting models and innovative, chain-linking based dasymetric population downscaling, including age-sex disaggregations, as well as global historical gridded population data from 1900 onwards produced by integrating historical, long-term land-use models with data from the Global Human Settlement Layer.

For robust and transparent gridded population data production, uncertainty awareness and -quantification is key. Hence, at the JRC, we explore novel ways to conduct accuracy assessments of gridded population data. For example, we benchmark our datasets against increasingly available authoritative gridded population and other official data reported by national census agencies, and develop new metrics tailored to estimate the accuracy of gridded population data and similar datasets in meaningful and intuitive ways. In our talk, we will highlight recent methodological advances on gridded population data quality assessments and showcase exemplary results of benchmarking and cross-comparing different gridded population datasets. Moreover, we will reflect on pitfalls and caveats that may occur when gridded population data accuracy assessments involve unsuitable data processing or sampling design and highlight the importance of reflected considerations of the fitness-for-use of these datasets.

How to cite: Uhl, J., Schiavina, M., Pigaiani, C., Batista e Silva, F., Alessandrini, A., Freire, S., Krasnodębska, K., Carioli, A., Pesaresi, M., Kemper, T., and Dijkstra, L.: Advances in producing and evaluating gridded population data at the European Commission’s Joint Research Centre, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20475, https://doi.org/10.5194/egusphere-egu26-20475, 2026.

EGU26-20620 | ECS | Orals | ITS1.14/GI1

Machine learning tools for estimating visitation to natural spaces in the UK 

Elizabeth Galloway, Yueyue Chai, Pippa Langford, and Peter Challenor

Protecting and restoring natural spaces is critical in the face of climate risks and environmental change, whilst at the same time, access to natural space plays an important role in population health and well-being. Understanding visitation patterns to natural spaces aids planning, maintenance, and land use, and allows us to evaluate the impact of interventions designed to benefit both nature and society. While surveys can provide snapshots of information about visits to natural spaces, robustly measuring visitor patterns on broad scales remains a challenge. Moreover, we lack the tools required to provide visitation estimates under the range of scenarios involved in land use and natural space planning. In this research, we develop scalable tools to predict visitor counts along paths in the UK located in natural spaces using Machine Learning methods, expanding on previous work by the Office for National Statistics. We employ a range of linear, tree-based, and time series models trained on automated footplate counter data and test our models across a range of spatial and temporal scenarios. Our models demonstrate promising ability to replicate historical visitation patterns at many sites, suggesting data-driven methods could offer valuable insights into the sustainable management of natural spaces. We also highlight areas for future improvement, such as improving the spatial generalisability of the models, which could inform future visitation monitoring strategies. Finally, we use Explainable AI approaches to investigate the characteristics of natural space visitation, providing information for planning and interventions which we explore in this study using a storytelling approach.

How to cite: Galloway, E., Chai, Y., Langford, P., and Challenor, P.: Machine learning tools for estimating visitation to natural spaces in the UK, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20620, https://doi.org/10.5194/egusphere-egu26-20620, 2026.

Nature-based recreational activities are highly sensitive to climate change. Particularly, hiking tourism is exposed to weather and climate variability that can affect the accessibility and attractiveness of trekking routes and alter tourism seasonality and flows. Thus, there is an urgent need for climate adaptation actions for effectively responding to climatic and environmental pressures and ensuring continuity of outdoor tourism experiences.

So far, responses within the tourism sector have been largely managed by individual operators, through unsustainable coping measures aimed at managing climate variability and related shifts in supply and demand patterns. Integrated approaches that could promote more effective, long-term climate adaptation, while enhance landscape heritage resources and prioritize the needs of the local community remain weak and isolated. This challenge is even more pressing in rural communities where nature-based tourism is envisioned as a sustainable driver for economic revitalization and socio cultural innovation against depopulation and aging. However, they frequently lack adequate resources, institutional support, and policy frameworks to implement effective adaptation strategies, while short-term management decisions and low public awareness further exacerbate vulnerabilities.

This contribution presents a participatory adaptive planning approach for nature-based tourism in rural contexts. The case study involves six small municipalities in the Fiastra river valley (Marche region, Italy), where a cultural trekking route – the Anello della Val di Fiastra – has been developed to promote responsible territorial enhancement by combining slow tourism, unique natural landscapes and the local cultural heritage. A scenario-based planning workshop was organized to engage stakeholders in discussing plausible future climate conditions for thevalley. Participants were projected to the year 2068, characterized by rising temperatures, increased frequency of heatwaves and tropical nights, and more intense rainfall events. They were asked to identify landscape assets most at risk and to co-design adaptive solutions to preserve territorial attractiveness and ensure the walkability of the route throughout the year. Environmental hiking guides, tourism operators, heritage managers, and representatives of local cultural associations collectively mapped vulnerable and exposed places along the route and discussed potential responses, spatializing them where possible. Proposals ranged from long-term strategies to operational measures and tactical interventions, including nature-based and engineering solutions, financial instruments, tourism supply management, training and awareness-raising initiatives, and governance actions.

The workshop was conducted within the newly established landscape observatory of the Fiastra Valley, a local entity studying landscape dynamics and risk conditions towards bettermanagement policies. Findings provide insights into the actors and planning instruments required for effective adaptive decision-making in nature-based tourism. Moreover, this studyhighlights the value of community-based and interdisciplinary research in fostering mutual learning and co-creation of knowledge, by redefining spaces and modes of relationship between local authorities and actors for risk management and climate adaptation.

The research is part of the project “QUI Val di Fiastra”, funded by the Italian National Recovery and Resilience Plan, Intervention 2.1 – Attractiveness of historic villages.

How to cite: Baldassarre, B., De Luca, C., Giacomelli, M., and Barchetta, L.: Participatory adaptive planning for nature-based tourism in a changing climate: the case of “Anello della Val di Fiastra” hiking path, Marche region, Italy , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20623, https://doi.org/10.5194/egusphere-egu26-20623, 2026.

EGU26-20901 | ECS | Orals | ITS1.14/GI1

The environmental and health impacts of diets and dietary change in 5,500 cities worldwide 

Sebastiano Caleffi, Marco Springmann, Jack Rawden, and Olivia Auclair

The majority of the world’s population live in cities, making urban food environments an important driver of global diets and their associated health and environmental impacts. However, only a few dietary and food-system assessments have been conducted at the city level, often with important shortcomings which limit consistent policy planning. Existing studies cover only a few cities and mostly large ones, leaving many smaller cities without estimates. Further, most simply scaled national estimates of food intake – either from food balances or surveys – to city populations. We combined dietary data for urban residences by age and sex, gridded age and sex structures from WorldPop, and urban settlement polygons from the Global Urban Polygons and Points Dataset (GUPPD), to estimate the dietary intake in 5,500 cities with populations over 100 thousand inhabitants. Our estimates indicate that diets in most cities contained greater amounts of foods compared to a country’s average intake in 2020. As a result, cities in most regions were responsible for a larger share of food-related environmental resource use and pollution compared to their share of population. This was mostly driven by increased intake of animal source foods in cities included in our impact assessment. Cities were also responsible for a large share of diet-related health burden and an outsized share of health-related costs, in line with the generally higher cost levels observed in cities. Dietary changes to healthier and more sustainable diets could substantially reduce the environmental, health, and cost impacts associated with city diets, but are dependent on consistent policy approaches and support.

How to cite: Caleffi, S., Springmann, M., Rawden, J., and Auclair, O.: The environmental and health impacts of diets and dietary change in 5,500 cities worldwide, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20901, https://doi.org/10.5194/egusphere-egu26-20901, 2026.

The valorization of intangible cultural heritage represents a cornerstone for developing resilient
and sustainable tourism models in rural areas. Within the framework of the transborder project
CulinaryTrail.eu, this study focuses on the Gagauzia region (Republic of Moldova), a unique
cultural enclave in the Danube basin. Our research aimed to identify, document, and inventory
specific culinary assets that define the identity of the Gagauz community and assess their potential
to catalyze Community-Based Sustainable Tourism (CBST).
The methodology integrated ethnographic field research, semi-structured interviews with local
practitioners, and participatory mapping. The resulting inventory comprises 20 distinct units of
culinary heritage, classified into traditional dishes (e.g., kaurma, gözleme), specific processing
techniques (such as the use of traditional ovens and clay vessels), local beverages, and communitydriven
gastronomic events.
The analysis reveals that these culinary assets are not merely food products, but "living artifacts"
that encode migration history, adaptation to the steppe environment, and social cohesion. We
argue that the systematic integration of this inventory into the Culinary Trail network can:
Redirect tourist flows from oversaturated centers toward the Danubian hinterland—a
territory that remains peripheral yet profoundly authentic;
Ensure economic circularity by establishing direct links between small-scale local producers
and the regional hospitality sector;
Safeguard local biocultural identity by revitalizing authentic recipes and indigenous
ingredients.
The findings presented in this work demonstrate how a data-driven culinary inventory serves as a
vital tool for policymakers and local stakeholders in designing a tourism product that is both
economically viable and culturally respectful.
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How to cite: Căpățînă, L. and Odnostalco, I.: Mapping the Culinary Heritage of the Bugeac Steppe: A Strategic Inventory for Community-Based Sustainable Tourism in Gagauzia(Republic of Moldova), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21259, https://doi.org/10.5194/egusphere-egu26-21259, 2026.

European coastal regions represent a substantial share of the European tourism economy, but they are also among the places where climate change is most likely to be felt by visitors and businesses alike. Rising temperatures, changing precipitation regimes, and altered wind and cloudiness patterns can directly affect thermal comfort and perceived “beach quality,” with implications for visitation, seasonality, and local economies. This study quantifies how climate shapes coastal-beach tourism demand across Europe and translates these relationships into forward-looking, risk-based scenario insights.

Climate suitability is characterized using the Holiday Climate Index for beach tourism (HCI:Beach; Scott et al., 2016), a bioclimatic indicator integrating temperature, precipitation, humidity, wind, and cloudiness to reflect tourists’ stated preferences and destination comfort. This indicator is employed in a monthly panel tourism-demand model estimated on historical regional observations of tourism activity, alongside sector-specific controls and fixed effects. The resulting estimates indicate a statistically significant link between HCI:Beach and tourism demand, and a clear north-south pattern in demand changes in observed , with northern regions benefiting and southern regions experiencing significant reductions, particularly in higher warming scenarios.

To evaluate future impacts, monthly HCI:Beach projections through 2100 are generated using an ensemble of ten regional climate models, and corresponding changes in tourism demand are simulated. Uncertainty is represented from two sources: (i) climate model spread, by sampling across the ensemble projections of the underlying climate variables, and (ii) statistical uncertainty, by repeatedly drawing from the estimated parameter distribution of the demand model. These components are combined in a Monte Carlo framework, producing distributions of future demand outcomes.

Results are reported under two emissions pathways (RCP4.5 and RCP8.5) and, to support policy-relevant interpretation, are also summarized for four global warming levels (1.5°C, 2°C, 3°C, and 4°C). Across European coasts, projections reveal strong spatial and seasonal heterogeneity: climate change can improve suitability in some destinations and months (often in shoulder seasons) while degrading peak-season conditions elsewhere, implying shifts in the timing and geography of demand.

The risk assessment translates probabilistic projections into decision-ready metrics, such as the probability of peak-season demand losses exceeding specified thresholds, the likelihood of shoulder-season demand gains, and the emergence of “high-risk months” in which unfavorable beach conditions become consistently more common. Robust signals are further identified (high agreement across climate models and stable econometric effects) versus deep-uncertainty cases where adaptive strategies should remain flexible.

Finally, building on these findings, adaptation options tailored to regional and seasonal risk profiles are discussed, including spreading demand though season extension and product diversification, or managing heat and comfort through services and information. By integrating a preference-based climate index, econometric demand estimation, multi-model climate projections, and probabilistic risk metrics, this study provides a transparent framework to anticipate where, when, and how European coastal tourism may change.

Keywords: climate change impacts, coastal tourism demand, panel data analysis, HCI:Beach (Holiday Climate Index)

How to cite: Matei, N. A.: Tides of Change: How Climate Will Reshape Coastal Tourism in Europe. Destination Shifts, Economic Impacts, and Adaptation Options, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21281, https://doi.org/10.5194/egusphere-egu26-21281, 2026.

EGU26-2491 | Orals | MAL16-GI | Christiaan Huygens Medal Lecture

The Fractal Nature of the Earth: Redefining Geophysical Interpretation 

Vijay Prasad Dimri

Sources of geophysical anomalies, such as density, susceptibility, conductivity, reflectivity, etc., are not always random as we often assume, but follow a scaling/fractal distribution. This has been demonstrated by analyzing borehole data from the German Continental Deep Drilling Programme (KTB) and other boreholes used for oil exploration. The new scaling spectral method (SSM) was developed to interpret gravity, magnetic, resistivity, and other geophysical measurements, which are better than the conventional spectral method. The application of fractal and scaling approaches in Earth science is widespread across all aspects of geophysics, including the acquisition, processing, and interpretation of geophysical data. The selection criteria for spacing for measurement stations in a 1D survey or grid size for a 2D survey have been suggested. Similarly, processing of non-stationary data is subdivided into stationary data for which the SSM can be applied. Potential field theory has also been studied in the context of fractals or scaling laws and has been found to be worthwhile in inferring the physical properties of the subsurface. The Voronoi tessellation approach using fractional dimension has been applied to model the subsurface from field geophysical data. Here, an attempt is made to discuss the in-depth review of the application of the fractal/scaling approach for qualitative and quantitative interpretation of complex sources of interest. The implications of this study will be beneficial for readers, enabling them to understand the gaps in subsurface source characterization, with practical applications demonstrated through field geophysical examples. 

How to cite: Dimri, V. P.: The Fractal Nature of the Earth: Redefining Geophysical Interpretation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2491, https://doi.org/10.5194/egusphere-egu26-2491, 2026.

EGU26-12462 | ECS | Orals | MAL16-GI | GI Division Outstanding ECS Award Lecture

Potential field theory for ground deformation: a new tool for the space-borne monitoring of volcanoes and fluid reservoirs. 

Andrea Barone

Ground deformation fields are widely recognized as key tools for the study of geological phenomena such as volcanic eruptions, which cause displacements in the Earth’s surface and interior. When ground deformation data are available, modeling approaches enable the characterization of deformation sources, such as overpressurized and migrating volcanic or hydrothermal fluids within the crust. Geodetic data modeling is therefore a powerful approach for monitoring volcanic systems, managing alerts, and mitigating possible disasters.

For the characterization of ground deformation, the satellite-based Interferometric Synthetic Aperture Radar (InSAR) technique now plays a significant role, as it provides high-quality spaceborne data with extensive coverage and varying resolution. Moreover, several technological efforts are currently ongoing within the Earth Observation framework to advance SAR sensors and related satellite missions, as well as to refine data systems in order to automatically provide measurements of the Earth’s surface deformation in near real time. However, these advancements have not yet been matched by comparable progress in geodetic data modeling strategies. Indeed, the most commonly used modeling approaches, based on parametric optimization and tomographic inversion algorithms, are often unable to address the inherent issues of inverse problem solutions. In addition, they rarely guarantee a reliable characterization of the volcanic context, as they rely on several assumptions underlying analytical models. Finite Element (FE) approaches can potentially ensure greater reliability, although the number of variables to be managed and the computational cost increase considerably. As a result, modeling strategies may fail to determine a unique solution for source parameters when adequate model constraints are not available.

This research topic aims to address ambiguities in the modeling of volcanic deformation sources in order to ensure the full exploitation of the large amount of available InSAR data. This task requires methods capable of providing unambiguous constraints on source parameters while being fast, computationally efficient, and easy to implement in automatic modeling tools, making them suitable for monitoring systems. Our proposal is based on imaging and multiscale methods of potential fields, which satisfy these requirements, even though the deformation field itself is not formally defined as a potential field.

Here, we demonstrate that, under certain conditions, potential field theory can be applied to analyze deformation fields, which can be expressed through harmonic and homogeneous functions. During the lecture, we present several tests validating the proposed arguments and discuss the usefulness of potential field theory in addressing different real-world cases (e.g., Campi Flegrei caldera, Yellowstone caldera, Okmok volcano, Uturuncu volcano, and Fernandina and Sierra Negra volcanoes), using Multiridge and ScalFun methods to constrain the geometric parameters of magmatic reservoirs, boundary analysis techniques to image medium heterogeneity, and potential function evaluation to reconstruct the three-dimensional displacement field.

The results highlight that the proposed methodological suite meets all the necessary requirements to improve the geodetic modeling of volcanic systems and can be integrated into monitoring facilities as an automatic and efficient tool.

How to cite: Barone, A.: Potential field theory for ground deformation: a new tool for the space-borne monitoring of volcanoes and fluid reservoirs., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12462, https://doi.org/10.5194/egusphere-egu26-12462, 2026.

EGU26-5340 | ECS | Posters virtual | VPS21

A Multi-Objective Cost Minimization Framework for Managed Aquifer Recharge Integrating Pareto Optimization and Least-Cost Path Analysis 

Rahma Fri, Andrea Scozzari, Souad Haida, Malika Kili, Jamal Chao, Abdelaziz Mridekh, and Bouabid El Mansouri

In arid and semi-arid regions, pressure on groundwater resources has reached critical levels. Long-term over-pumping has depleted many aquifers, and climate change is intensifying this process. Rising temperatures increase evaporation from rivers and reservoirs, reducing the amount of surface water available for infiltration and natural recharge. Under these conditions, the use of surface water during periods of availability and its storage underground represents a key mechanism of managed aquifer recharge, effectively avoiding evaporation losses.

In this study, a practical framework is developed and tested to identify feasible ways to transfer accumulated surface water toward stressed aquifers. Rather than relying on complex ranking approaches, the locations of existing water infrastructure specifically wells and traditional khettara systems are used as reference points. These features indicate where aquifers are accessible and provide realistic spatial anchors for planning recharge at the regional scale.

The method combines satellite imagery to map surface water, geographic information systems (GIS) to identify cost-effective transfer pathways across the landscape, and multi-objective optimization to evaluate trade-offs between competing objectives. Feasibility is assessed through a cost function that accounts for terrain slope, elevation differences, transfer distance, pumping energy requirements, infrastructure costs, and potential water treatment needs.

The approach is applied to the Draa Oued Noun Basin in southern Morocco, a region strongly affected by water scarcity, high evaporation rates, and declining groundwater levels. Several surface water sources are examined, and feasible conveyance routes toward aquifers supplying key wells and khettara systems are identified.

The results show substantial variations in cost between water sources. Available water volume, transfer distance, and especially elevation lift emerge as the main cost drivers. Trade-off analysis helps identify the most cost-effective projects under limited budgets. The results also highlight opportunities for cost reduction: where gravity-driven transfer is possible, costs are significantly lower, and where pumping is required, solar energy offers a viable option for reducing long-term operational expenses.

Overall, this work provides a spatially explicit and realistic basis for planning artificial groundwater recharge, while respecting economic constraints and supporting sustainable groundwater management in highly water-stressed regions.

 

 

How to cite: Fri, R., Scozzari, A., Haida, S., Kili, M., Chao, J., Mridekh, A., and El Mansouri, B.: A Multi-Objective Cost Minimization Framework for Managed Aquifer Recharge Integrating Pareto Optimization and Least-Cost Path Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5340, https://doi.org/10.5194/egusphere-egu26-5340, 2026.

EGU26-11154 | ECS | Posters virtual | VPS21

Choosing an I/O approach for Earth system models: lessons learned from a modular I/O server for MESSy 

Aleksandar Mitic, Patrick Jöckel, Astrid Kerkweg, Kerstin Hartung, Bastian Kern, and Moritz Hanke

Modern Earth system models increasingly hit I/O limits—not only in performance, but also in reproducibility, maintainability, and developer productivity. As data volumes and workflows evolve, tightly coupled, file-centric I/O approaches can become hard to scale and hard to extend.

We present the design and lessons learned from introducing an asynchronous, modular I/O server concept in the Modular Earth Submodel System (MESSy). I/O operations were decoupled from the Fortran-based scientific core and implemented as separate Python services, where the communication between the two components was implemented using the Yet Another Coupler (YAC) library. This architecture was chosen to improve flexibility and long-term maintainability, while enabling heterogeneous workflows and evolving storage backends.

Using MESSy as a case study, we discuss practical decision criteria for selecting an I/O concept in large models (e.g., scaling behavior, accessibility for developers, testing and CI strategies, and reproducibility).  We conclude with lessons learned from bridging Fortran and Python communities and from lowering entry barriers for user-developers in a large modeling system.

How to cite: Mitic, A., Jöckel, P., Kerkweg, A., Hartung, K., Kern, B., and Hanke, M.: Choosing an I/O approach for Earth system models: lessons learned from a modular I/O server for MESSy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11154, https://doi.org/10.5194/egusphere-egu26-11154, 2026.

EGU26-13270 | Posters virtual | VPS21

Integrating Participatory Perception-Mapping Data and Stochastic Image Analysis for Urban Landscape Assessment 

Stavroula Kopelia, Nikos Tepetidis, Julia Nerantzia Tzortzi, G.-Fivos Sargentis, and Romanos Ioannidis

Modern digital technologies and geoinformatics have experienced rapid growth, offering powerful tools to bridge the gap between scientific communities and society in landscape assessment and mapping. This research details the application of a crowdsourcing scheme that utilizes a dedicated mobile application to facilitate direct public participation in quantifying perceptions of urban landscapes and architecture. Initially developed as an educational tool, the methodology has been tested by university students across Italy, Greece, and France, providing a foundational phase for assessing landscape quality and urban typologies. Building upon these educational pilot studies, the work explores the evolution of this methodology into a broader, multicultural citizen science initiative designed to improve the quality and quantity of available landscape perception data.

A significant technical advancement in this research involves the integration of automated image analysis to process the novel data generated by participants from any location. The photographic material was examined using stochastic image analysis based on climacograms, in which images are treated as two-dimensional grayscale intensity fields and analyzed across multiple spatial scales. The method enables the comparison of image patterns based on the visual complexity of the uploaded photographs. A primary challenge addressed was the algorithm's performance when processing real-world, non-curated smartphone images. The analysis began an assessment on how the methodology handles environmental noise, such as sky, trees, and unconventional capture angles, which are inherent to bottom-up crowdsourcing schemes.

The early results indicate that the method can reveal group-level tendencies associated with differing architectural characteristics, particularly in relation to visual complexity, while not supporting reliable classification at the level of individual image. In detail, the findings indicate a trend towards two categorizations: firstly, between modernist-type movements, characterized by minimal elements, and secondly between eclectic or decorative movements, which exhibited higher measured complexity; however, this this behaviour was not observed universally on all analyzed movements The stochastic analysis also indicated theoretical overlaps between certain movements, such as Postmodernism and Eclecticism, based on shared decorative patterns. While the results highlight that environmental factors can influence the analysis of individual photographs, the method utilized presents potential for distinguishing movement trends with logical consistency even from unfiltered data.

Scientifically, this yield of quantitative data sets the groundwork for improved research in the humanities and culture, showing a strong correlation with established landscape quality indices. Socially, the project provides a scalable model for participatory mapping that fosters critical thinking about urban quality, creating new conditions for communication between universities and the broader public. Overall, the presented work reports on the early-stage results of this methodological exploration and aims to evaluate the combined use of participatory mobile data collection and exploratory image-based analysis for landscape and architectural studies, while identifying key challenges related to data quality, interpretation, and future methodological refinement.

How to cite: Kopelia, S., Tepetidis, N., Tzortzi, J. N., Sargentis, G.-F., and Ioannidis, R.: Integrating Participatory Perception-Mapping Data and Stochastic Image Analysis for Urban Landscape Assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13270, https://doi.org/10.5194/egusphere-egu26-13270, 2026.

EGU26-13783 | Posters virtual | VPS21

Monitoring Land Cover Dynamics in Bahr Qarun District, Egypt, via Remote Sensing Data  

Abdelrahman Elsehsah, Abdelazim Negm, Eid Ashour, and Mohammed Elsahabi

Accurate monitoring of land cover is essential for sustainable environmental management and urban planning in arid regions. However, rapid changes in land use often make it difficult to distinguish between different surface types, such as urban areas and bare soil, using standard satellite data alone. This research examines land-use changes in the Bahr Qarun district of Fayoum, Egypt, during 2019, 2021, and 2023. The study used Sentinel-2 and Landsat OLI 8 satellite images taken each April to ensure data consistency. We applied the Maximum Likelihood (ML) method to classify Sentinel-2 images. They used 30 training samples for each land category to guide the process. The results achieved a Kappa coefficient above 75%, indicating a reliable level of accuracy. We measured vegetation using the Normalized Difference Vegetation Index (NDVI) and urban areas using the Normalized Difference Built-up Index (NDBI). A comparative analysis revealed that NDVI results were closely aligned with those obtained from supervised classification, reflecting its strong capability in accurately identifying vegetated areas. In contrast, NDBI exhibited a tendency to overestimate urban extent, primarily due to spectral confusion between built-up surfaces and bare soil within individual pixels. The study concludes that NDVI is an effective tool for mapping the green cover in this area.

Keywords: Land Cover Change, Sentinel-2, Landsat OLI 8, Supervised Classification,  Spectral Indices (NDVI & NDBI), Bahr Qarun, Egypt.

How to cite: Elsehsah, A., Negm, A., Ashour, E., and Elsahabi, M.: Monitoring Land Cover Dynamics in Bahr Qarun District, Egypt, via Remote Sensing Data , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13783, https://doi.org/10.5194/egusphere-egu26-13783, 2026.

EGU26-13852 | ECS | Posters virtual | VPS21

Monitoring Shallow Water Depths: A Review of Satellite-Derived Bathymetry Methods 

Mohamed H. Abdalla, Hassan Elhalawany, Saad M. Abdelrahman, Abdelazim Negm, and Andrea Scozzari

Satellite-Derived Bathymetry (SDB) offers a cost-effective alternative to traditional shipborne surveys for mapping large coastal areas. This technique utilizes optical remote sensing data from multispectral sensors to estimate water depth. The fundamental principle relies on the behavior of light as it travels through the water column; as depth increases, light intensity decreases due to absorption and scattering. Different wavelengths penetrate to varying degrees, with blue light reaching the greatest depths while red light is absorbed quickly. By analyzing these spectral features, researchers can calculate underwater topography. Currently, SDB techniques are categorized into two primary groups: physically based (analytical) models, which simulate light propagation without needing local in-situ depth calibration, and statistical (empirical) models, which correlate satellite data with known depth measurements from nautical charts, ship-based acoustic surveys or airborne LiDAR.

While both approaches provide extensive spatial coverage at a lower cost, they are generally limited to clear, shallow waters, typically reaching depths of less than 20 meters. Analytical models are highly accurate but complex and data-intensive, whereas empirical models are more accessible but rely heavily on the quality of reference data. Recent advancements in machine learning have significantly improved the automation and performance of these empirical methods. This study evaluates the core concepts, advantages, and limitations of various SDB approaches, with a focus on Landsat-8 and Sentinel-2 data. Furthermore, the research details essential processes for empirical model calibration, validation, and detecting model bias. The findings emphasize that rigorous evaluation and bias correction are critical for ensuring the reliability of depth data in diverse coastal environments.

Keywords: Satellite-Derived Bathymetry, Remote Sensing, Empirical Models, Stumpf Algorithm, Coastal Waters, Model Bias Detection and Correction.

How to cite: Abdalla, M. H., Elhalawany, H., Abdelrahman, S. M., Negm, A., and Scozzari, A.: Monitoring Shallow Water Depths: A Review of Satellite-Derived Bathymetry Methods, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13852, https://doi.org/10.5194/egusphere-egu26-13852, 2026.

EGU26-19784 | Posters virtual | VPS21

Operationalising Semantic Interoperability for Cross-domain Discovery with LUMIS 

Julien Homo, Christelle Pierkot, Kévin Darty, and Hakim Allem

Significant heterogeneity in metadata schemas, vocabularies, and ontologies hinders the discovery, reuse, and integration of European environmental data infrastructures across national and disciplinary boundaries. Recent initiatives have identified semantic interoperability as a vital enabler of FAIR data flows between infrastructures, paving the way for sophisticated, AI-driven, large-scale analyses.

Powered by OntoPortal technology, EarthPortal is a specialised catalogue of semantic resources (ontologies, thesauri and controlled vocabularies) for Earth and environmental sciences. It provides navigation, multi-ontology searching, mapping management, text annotation and recommendation services via web interfaces and REST APIs. These support data catalogues and repositories in an interoperable way.

EOSC LUMEN builds an interoperable discovery ecosystem across multiple domains (including Earth System Science, Social Sciences and Humanities, and Mathematics) to enable cross-platform search and meaningful reuse across communities. Rather than focusing only on metadata aggregation, LUMEN targets the practical enablers of interoperability that make resources discoverable and machine-actionable across infrastructures.

LUMIS (LUMEN Infrastructure for Semantics) is the shared semantic layer of LUMEN. It supports the end-to-end lifecycle of semantic artefacts (ontologies and controlled vocabularies, including SKOS resources) from scoping and requirements to implementation, publication and long-term maintenance. LUMIS focuses on governance, provenance, versioning and quality checks, while adopting an integration-first strategy: it connects and orchestrates established community tools (deployed services and/or API-based components) into coherent workflows, so that semantic resources can be created, aligned, validated and delivered in reusable forms for discovery platforms.

Integrating EarthPortal into LUMIS links a domain-specific semantic catalogue to a cross-domain discovery ecosystem. This enables repositories to annotate metadata using EarthPortal resources, while making use of LUMIS’s lifecycle-driven workflows and FAIR-aligned governance and quality checks.

In this presentation, we will demonstrate how integrating EarthPortal into the LUMIS platform supports more consistent semantic interoperability and FAIR-aligned practices across European Earth System Science infrastructures. We will showcase practical data workflows to enhance interdisciplinary research.

How to cite: Homo, J., Pierkot, C., Darty, K., and Allem, H.: Operationalising Semantic Interoperability for Cross-domain Discovery with LUMIS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19784, https://doi.org/10.5194/egusphere-egu26-19784, 2026.

EGU26-20391 | Posters virtual | VPS21

A Scalable, FAIR‑Aligned Data Lake Architecture for Earth System Modelling: From Heterogeneous Raw Archives to Curated, Metadata‑Rich, Analysis‑Ready Climate Data 

Bushra Amin, Jakob Zscheischler, Luis Samaniego, Jian Peng, Almudena García-García, and Toni Harzendorf

Modern Earth system research relies on integrating heterogeneous datasets such as reanalysis, satellite observations, in situ measurements, climate model ensembles, and reforecasts, yet these data are often stored in fragmented, inconsistent, and difficult to reuse forms. This limits reproducibility, slows modelling workflows, and constrains the development of operational digital twins for water and climate risk management.

This contribution presents a scalable, FAIR aligned data lake architecture implemented on the EVE high performance computing environment. The system transforms a large, unstructured source pool of more than two million files into a curated, duplication free, metadata rich repository designed for hydrological modelling, machine learning, and climate analytics. The architecture follows a four stage lifecycle: raw, curated, database ready, and ancillary GIS layers, reflecting data governance practices used by major climate centres.

A reproducible ingestion workflow classifies, deduplicates, and standardizes datasets from ERA5, ERA5 Land, MERRA 2, PRISM, E OBS, GPM IMERG, CMIP6, ISIMIP3, ECMWF reforecasts, MODIS, CHIRPS, GFED, GRDC, GSIM, and other sources. A Python based metadata extractor, built on CF convention standards, automatically captures variables, units, dimensions, spatial resolution, temporal coverage, coordinate reference systems, and checksums. Metadata are stored both as dataset level JSON and as a global inventory, enabling transparent provenance tracking and rapid dataset discovery.

The curated data hub is implemented under /data/db/earth_system and organized by scientific domain, temporal resolution, spatial extent, and processing stage. The system supports SLURM based workflows, HPC native processing, and cloud optimized formats such as Zarr.

This work demonstrates how a single researcher can design and operationalize a modern, HPC native data infrastructure that accelerates hydro climate research and forms the backbone of an emerging Digital Hydro Twin. The approach is transferable to institutions seeking to modernize their data ecosystems and improve reproducibility in environmental modelling.

How to cite: Amin, B., Zscheischler, J., Samaniego, L., Peng, J., García-García, A., and Harzendorf, T.: A Scalable, FAIR‑Aligned Data Lake Architecture for Earth System Modelling: From Heterogeneous Raw Archives to Curated, Metadata‑Rich, Analysis‑Ready Climate Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20391, https://doi.org/10.5194/egusphere-egu26-20391, 2026.

EGU26-21793 | Posters virtual | VPS21

Hydrological Modelling of the Upper Senegal River Basin Using SWAT: Assessing the Impact of Multi-Source Precipitation Data on Model Performance 

Sidi Mohamed Boussabou, Soufiane Taia, Bouabid El Mansouri, Aminetou Kebd, Abdallahi Mohamedou Idriss, Hamza Legsabi, and Lamia Erraioui

The Upper Senegal River Basin is a strategic water resource system supporting agriculture, hydropower generation, and essential ecosystem services in West Africa. However, a comprehensive understanding of its hydrological dynamics remains constrained by the limited availability of in situ hydroclimatic observations. This study applies the Soil and Water Assessment Tool (SWAT) to simulate hydrological processes in the basin, with a particular emphasis on the influence of precipitation data sources on model performance and uncertainty. Hydrological simulations were conducted at six representative gauging stations (Bakel, Kayes, Gourbassy, Oualia, Bafing Makana, and Daka Saidou) over the period 1983–2021, using a combination of ground-based observations, satellite precipitation products, and reanalysis datasets (ERA5, MERRA-2, PERSIANN, and CHIRPS). Model calibration demonstrated satisfactory performance, with Nash–Sutcliffe Efficiency (NSE) values reaching up to 0.74 at upstream stations, while reduced performance was observed downstream. Validation results showed a moderate decline in model efficiency, highlighting the sensitivity of SWAT outputs to precipitation inputs and data uncertainty. The comparative analysis of precipitation datasets reveals substantial variability in simulated streamflow and water balance components, underscoring the importance of precipitation data selection in data-scarce regions. These findings highlight the need for robust, multi-source hydroclimatic data integration to improve hydrological modelling reliability and support informed water resource management decisions.

Keywords: Upper Senegal River, SWAT, Hydrological modelling, Precipitation uncertainty; Satellite rainfall; Reanalysis data.

How to cite: Boussabou, S. M., Taia, S., El Mansouri, B., Kebd, A., Mohamedou Idriss, A., Legsabi, H., and Erraioui, L.: Hydrological Modelling of the Upper Senegal River Basin Using SWAT: Assessing the Impact of Multi-Source Precipitation Data on Model Performance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21793, https://doi.org/10.5194/egusphere-egu26-21793, 2026.

EGU26-21965 | Posters virtual | VPS21

An EOSC Node Ireland Pilot Study: Bridging European and National e-Infrastructures for Reproducible Sentinel-2 Data Ingestion in Quarry Applications 

Flaithri Neff, Roberto Sabatino, Alfredo Arreba, and Jerry Sweeney

The establishment of the European Open Science Cloud (EOSC) places renewed emphasis on the role of national e-infrastructures in enabling standards-based, interoperable, and reusable research workflows in the EU. Within the context of Ireland’s EOSC Node, there is particular interest in demonstrating how European-scale open-data services can be digested by national research clouds, transformed into analysis-ready assets, and made available for both open research and applied industry use-cases. Earth Observation (EO) provides a strong test case, given the volume and complexity of the data involved, and its growing role in scalable environments that support operational decision-making.

This pilot project, QuarryLink, presents a Phase-1 study focused on building a reproducible EO data ingestion workflow that connects the Copernicus Data Space Ecosystem with the HEAnet Research Cloud, operating on the SURF Research Cloud platform. Through a real-world quarry case-study in the Dublin region (Ireland), the work demonstrates how EOSC-aligned principles, including auditable machine-readable workflows, can be applied from the outset of the EO research process. We will demonstrate how precise spatial boundaries can be defined and validated; how modern OAuth-based authentication mechanisms can be integrated into research cloud workflows; and how Sentinel-2 Level-2A products can be programmatically discovered, retrieved, and prepared for downstream analysis using current Copernicus services.

By executing the ingestion workflow on the HEAnet Research Cloud using open-source geospatial tooling, the pilot aims to establish an analytics-ready foundation for working with Sentinel-2 data in a reproducible research cloud environment. The resulting data products are structured to support downstream analysis, with compute resources accessed dynamically through the HEAnet Research Cloud workspace as required. Building on this foundation, Phase 2 will focus on developing time-series analyses, EO data cubes, and derived environmental indicators to support both research-driven investigation and applied monitoring scenarios in European quarry environments.

More broadly, the pilot seeks to illustrate how EOSC-aligned integration across data ingestion and compute layers can support open research practices while enabling scalable, real-world EO-enabled industrial applications, providing a practical pathway for national EOSC Nodes to translate open data into shareable analytics and societal impact.

How to cite: Neff, F., Sabatino, R., Arreba, A., and Sweeney, J.: An EOSC Node Ireland Pilot Study: Bridging European and National e-Infrastructures for Reproducible Sentinel-2 Data Ingestion in Quarry Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21965, https://doi.org/10.5194/egusphere-egu26-21965, 2026.

EGU26-22084 | ECS | Posters virtual | VPS21

Monitoring Groundwater Quality and Improvement in the Kima Area, Aswan 

Marwa Khairy, Ahmed S. Nour-Eldeen, Hickmat Hossen, Ismail Abd-Elaty, and Abdelazim Negm

Groundwater in arid regions is highly sensitive to human activity, especially when untreated wastewater interacts with shallow aquifers. This study evaluates the hydrogeochemical response of the Kima aquifer in Aswan, Egypt, following the Kima Drain Covering Project. The research uses an integrated framework of field measurements, geospatial analysis, and multi-criteria decision-making. The team analyzed groundwater samples from 2020 and 2025. They tested eleven physicochemical parameters and six irrigation indices. Spatial interpolation through Inverse Distance Weighting (IDW) helped map temporal variations and identify contamination hotspots. To classify water suitability, the study standardized values according to WHO and Egyptian guidelines. The Analytical Hierarchy Process (AHP) was used to determine the importance of various drinking and irrigation indicators. Finally, a Weighted Linear Combination (WLC) generated composite Groundwater Quality Index (GWQI) maps. The results show a significant improvement in groundwater quality after the drain was covered. Levels of TDS, chloride, sulfate, sodium, and magnesium decreased substantially across the area. The ionic balance shifted toward a more favorable calcium-magnesium-bicarbonate facies. Irrigation indices also improved, with most parameters falling into safe or excellent ranges. The 2025 GWQI map reveals a transition from "good–permissible" to "excellent–safe" zones. This confirms that eliminating direct seepage from the drain had a positive environmental impact. This integrated AHP–GIS–IDW approach is an effective tool for monitoring groundwater changes. It provides a robust decision-support system for managing water resources in arid urban environments.

How to cite: Khairy, M., S. Nour-Eldeen, A., Hossen, H., Abd-Elaty, I., and Negm, A.: Monitoring Groundwater Quality and Improvement in the Kima Area, Aswan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22084, https://doi.org/10.5194/egusphere-egu26-22084, 2026.

EGU26-3080 | ECS | Posters virtual | VPS22

Multibranch Adaptive Feature Fusion for Hyperspectral Image Classification 

Chen Li and Baoyu Du

Hyperspectral image (HSI) classification often struggles with feature interference across different scales and the inherent challenges of data imbalance and sample scarcity. While deep learning models have significantly advanced the field, traditional single-branch architectures often suffer from scale-related noise, where features from different receptive fields interfere with one another. To address this, we propose the Multibranch Adaptive Feature Fusion Network (MBAFFN). Our approach utilizes three parallel branches to independently extract scale-specific features, effectively decoupling the multiscale information to prevent interference. This architecture is enhanced by two specialized modules: Global Detail Attention (GDA) for capturing broad contextual dependencies and Distance Suppression Attention (DSA) for refining local pixel-level discrimination. Furthermore, a pixel-wise adaptive fusion mechanism is introduced to dynamically weigh and integrate these features, prioritizing the most relevant scales for final classification. The performance of MBAFFN was validated on four benchmark datasets: Indian Pines (IP), Pavia University (PU), Longkou (LK), and Hanchuan (HC). Compared to current state-of-the-art methods, our model improved Overall Accuracy (OA) by 0.91%, 1.71%, 0.86%, and 3.16% on the IP, PU, LK, and HC datasets, respectively. The significant improvement on the HC and PU datasets underscores the model’s robustness in scenarios with limited training samples and complex class distributions. These results, supported by detailed ablation studies, demonstrate that adaptive fusion and scale-specific branching are effective strategies for mitigating feature interference in hyperspectral analysis.

How to cite: Li, C. and Du, B.: Multibranch Adaptive Feature Fusion for Hyperspectral Image Classification, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3080, https://doi.org/10.5194/egusphere-egu26-3080, 2026.

EGU26-3363 | ECS | Posters virtual | VPS22

In-situ Thermal Infrared Monitoring in an Urban Area: A Case Study of Micro-scale Thermal Transitions during Hot Weather Conditions in Athens, Greece. 

Odysseas Gkountaras, Chryssoula Georgakis, Thiseas Velissaridis, and Margarita Niki Assimakopoulos

Characterizing the thermal state of urban surfaces is fundamental for mitigating the impacts of the Surface Urban Heat Island (SUHI) effect. This study presents an intensive in-situ thermal infrared monitoring campaign in the high-density urban core of Athens, Greece. Utilizing a calibrated handheld TIR sensor (7.5–14 μm), surface temperatures were recorded across strategic locations in the center of Athens during hot weather conditions. The methodology emphasizes the critical role of material-specific parameterization, where thermographic data were post-processed to account for emissivity (ε) variations and surface temperature, ensuring high-fidelity measurements.

Experimental results reveal extreme thermal stress, with maximum surface temperatures reaching 56.0°C on conventional paving materials, while the mean ambient air temperature was close to 35.0°C during peak solar hours (13:00–18:00LT). Spatial analysis and visualization of the results were performed using QGIS, correlating thermal signatures with urban geometry, shading conditions, and vegetation density. The aim of this study was to highlight the significant cooling potential of specific urban materials and nature-based solutions.

How to cite: Gkountaras, O., Georgakis, C., Velissaridis, T., and Assimakopoulos, M. N.: In-situ Thermal Infrared Monitoring in an Urban Area: A Case Study of Micro-scale Thermal Transitions during Hot Weather Conditions in Athens, Greece., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3363, https://doi.org/10.5194/egusphere-egu26-3363, 2026.

EGU26-3619 | ECS | Posters virtual | VPS22

Democratizing landslide detection for vulnerable regions beyond resource-intensive foundation models 

Rodrigo Uribe-Ventura, Willem Viveen, Ferdinand Pineda-Ancco, and César Beltrán-Castañon

Landslides claim thousands of lives and cause billions in economic losses annually, with impacts disproportionately concentrated in developing regions across Asia, Africa, and Latin America. Paradoxically, the current trajectory of artificial intelligence in geohazard detection—characterized by billion-parameter foundation models requiring substantial computational infrastructure—risks widening, rather than closing, the gap between technological capability and operational deployment where it is needed most. We argue that this paradigm requires fundamental reconsideration, proposing domain adaptation on strategically curated geological datasets as a more equitable and effective path toward globally accessible landslide detection systems.

Foundation models like the Segment Anything Model (SAM), pre-trained on over one billion masks, demand computational resources—312 million parameters, 1,376 GFLOPs per inference, specialized GPU infrastructure—that remain inaccessible to disaster management agencies in resource-constrained regions. Beyond these practical constraints, we contend that the apparent generalization capabilities of such models reflect pattern coverage in training data rather than emergent understanding transferable to geological contexts. The SA-1B dataset, despite its scale, was not curated to systematically represent landslide morphological diversity, creating coverage gaps for rare failure types, unusual triggering mechanisms, and underrepresented terrain configurations precisely where robust detection is operationally critical.

Given these limitations, we propose that effective generalization for geological applications emerges not from architectural scale but from strategic coverage of domain-relevant pattern space. We developed and tested GeoNeXt, a lightweight architecture that exploits the hierarchical transferability of geological features through targeted domain adaptation. Low-level representations (edges, spectral gradients) transfer universally across sensors and terrain; mid-level patterns (drainage networks, slope morphology) require adaptation to local expressions; and high-level configurations (failure geometries, trigger signatures) demand targeted training. Our results showed that this approach outperformed SAM-based methods across three independent benchmarks while requiring 10× fewer parameters (32.2M versus 312.5M) and a 62% reduction in computational cost. Zero-shot transferability to geographically distinct test sites (74–78% F1 score) emerged from the training dataset's systematic morphological diversity rather than parameter count. Inference at 10.6 frames per second on standard hardware, versus 3.0 frames per second for foundation model alternatives, transforms theoretical capability into deployable technology for resource-constrained environments. These findings suggest that strategic domain adaptation, rather than architectural scale, offers the most viable path toward operational landslide detection in vulnerable regions.

How to cite: Uribe-Ventura, R., Viveen, W., Pineda-Ancco, F., and Beltrán-Castañon, C.: Democratizing landslide detection for vulnerable regions beyond resource-intensive foundation models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3619, https://doi.org/10.5194/egusphere-egu26-3619, 2026.

EGU26-6022 | ECS | Posters virtual | VPS22

Geo2Gmsh: A Scalable Workflow for Automated Mesh Generation of Geological Models Using Gmsh 

Harold Buitrago, Juan Contreras, and Florian Neumann

Numerical modeling is a fundamental tool for understanding physically driven processes in geosciences. In multiparametric settings, the Finite Element Method is widely used because it can accommodate irregular geometries and complex boundary conditions. However, this advantage critically depends on the quality of the computational mesh, which must faithfully represent geological features such as faults, stratigraphic interfaces, and wells. In practice, mesh generation remains a major bottleneck, requiring specialized expertise and significant manual effort. We present Geo2Gmsh, an automated, lightweight workflow built on Gmsh (Geuzaine & Remacle, 2009), that generates geological meshes directly from simple text‐based descriptions of topological elements, including surfaces, lines, and points. These elements correspond to geologically meaningful features, allowing users to define faults, horizons, wells, and domain boundaries in a transparent, reproducible, and solver‐independent way. The workflow is demonstrated using two contrasting case studies: (1) Ringvent, an active sill‐driven hydrothermal system in the Guaymas Basin, and (2) the Eastern Llanos Basin, a foreland basin in eastern Colombia. To evaluate solver compatibility, we solved the heat equation in SfePy (https://sfepy.org/doc-devel/index.html) using the Eastern Llanos Basin model as the computational domain. Although the simulation is illustrative and not calibrated to observations, it confirms that meshes produced by Geo2Gmsh can be readily incorporated into numerical solvers. By explicitly embedding wells, faults, and geological interfaces in the mesh, Geo2Gmsh enables boundary conditions to be applied directly to physically meaningful features and allows model outputs to be extracted along them, simplifying both model setup and post‐processing. Meshes can be exported in standard formats (e.g., VTK, MSH, and Exodus via meshio), ensuring broad interoperability. Overall, Geo2Gmsh provides a lightweight, scalable, and reproducible workflow that dramatically lowers the technical barrier to geological mesh generation. This contribution establishes a practical foundation for reproducible, open-source numerical modeling in geosciences, facilitating the integration of geological knowledge into high-fidelity computational simulations.

How to cite: Buitrago, H., Contreras, J., and Neumann, F.: Geo2Gmsh: A Scalable Workflow for Automated Mesh Generation of Geological Models Using Gmsh, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6022, https://doi.org/10.5194/egusphere-egu26-6022, 2026.

EGU26-6232 | Posters virtual | VPS22

Application of advanced lossy compression in the NetCDF ecosystem for CONUS404 data 

Shaomeng Li, Allison Baker, and Lulin Xue

Many geoscientific datasets, such as those produced by climate and weather models, are stored in the NetCDF file format.  These datasets are typically very large and often strain institutional data storage resources. While lossy compression methods for scientific data have become more studied and adopted in recent years, most advanced lossy approaches do not work easily and/or transparently with NetCDF files. For example, they may require a file format conversion or they may not work correctly with “missing values” or “fill values” that are often present in model outputs.  While lossy quantization approaches such at BitRound and Granular BitRound have built-in support by NetCDF and are quite easy to use, such approaches are generally not able to reduce the data size as much as more advanced compressors (for a fixed error metric), like SPERR, ZFP, or SZ3.

We are particularly interested in reducing the data size of the CONUS404 dataset.  CONUS404 is a publicly available unique high-resolution hydro-climate dataset produced by Weather Research and Forecasting (WRF) Model simulations that cover the CONtiguous United States (CONUS) for 40 years at 4-km resolution (a collaboration between NSF National Center for Atmospheric Research the U.S. Geological Survey Water Mission Area). 

Here, we investigate one advanced lossy compressor, SPERR [1], together with its plugin for NetCDF files, H5Z-SPERR [2], in a Python-based workflow to compress and analyze CONUS404 data.  SPERR is attractive due to its support for quality control in terms of both maximum point-wise error (PWE) and peak signal-to-noise ratio (PSNR), enabling easy experimenting of storage-quality tradeoffs. Further, given a target quality metric, previous work has shown that SPERR likely produces the smallest compressed file size compared to other advanced compressors. It leverages the HDF5 dynamic plugin mechanism to enable users to stay in the NetCDF ecosystem with minimal to no change to existing analysis workflows, whenever a typical NetCDF file is able to be read. And, importantly for our work, the SPERR plugin supports efficient masking of “missing values,” which are common to climate and weather model output.  The support for missing values enables compression on many variables which are not naturally handled by other advanced compressors that rely on HDF5 plugins. Further, because H5Z-SPERR directly handles missing values, they can be stored in a much more compact format (and are restored during decompression), further improving compression efficiency. (Note that built-in NetCDF quantization approaches can work with missing values.) 

Our experimentation demonstrates the benefit of enabling advanced lossy (de)compression in the NetCDF ecosystem: adoption friction is kept at the minimum with little change to workflows, while storage requirements are greatly reduced.

 

[1] https://github.com/NCAR/SPERR

[2] https://github.com/NCAR/H5Z-SPERR

How to cite: Li, S., Baker, A., and Xue, L.: Application of advanced lossy compression in the NetCDF ecosystem for CONUS404 data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6232, https://doi.org/10.5194/egusphere-egu26-6232, 2026.

Investigations have been carried out into the initiation of the Pangu weather model, initiating the model with both ERA5 data (on which it was trained) and with the Met Office’s Global UM model data. There are many consistent local biases at ground level between these two sets of initial conditions. The geographically local biases are not dissipated by the Pangu model with timestep but instead remain geographically fixed and gradually decrease with lead time. Whilst the Pangu model initiated with UM initial conditions remains further from the ERA5 truth than the ERA5-initiated Pangu model at all timesteps, it initially moves towards the ERA5 truth with timestep, as the geographically static differences in initiation decrease, before moving further away from the ERA5 truth as differences in large-scale systems begin to dominate.

Also investigated was the difference between the Pangu model 24-hour timesteps and 6-hour timesteps; it was found that the 6-hour timesteps were better able to reduce the geographically static initial differences than the 24-hour timesteps.

If time permits, a similar analysis will be made of the FastNet and GraphCast models.

How to cite: Buttery, H.: Investigations into the Reaction of the Pangu ML Weather Model to Different Initial Conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7344, https://doi.org/10.5194/egusphere-egu26-7344, 2026.

EGU26-11945 | Posters virtual | VPS22

SEPNET: a multi-task deep learning framework for SEP forecasting 

Yang Chen, Yian Yu, Lulu Zhao, Kathryn Whitman, Ward Manchester, and Tamas Gombosi

Solar phenomena such as flares, coronal mass ejections (CMEs), and solar energetic particles (SEPs) are actively monitored and assessed for space weather hazards. In recent years, machine learning has demonstrated considerable success in solar flare forecasting. Accurate SEP forecasting remains challenging in space weather monitoring due to the complexity of SEP event origins and propagation. We introduce SEPNET, an innovative multi-task neural network that integrates forecasting of solar flares and CME summary statistics into the SEP prediction model, leveraging their shared dependence on space-weather HMI active region patches (SHARP) magnetic field parameters. SEPNET incorporates long short-term memory and transformer architectures to capture contextual dependencies. The performance of SEPNET is evaluated on the state-of-the-art SEPVAL SEP dataset and compared with classical machine learning methods and current state-of-the-art pre-eruptive SEP prediction models. The results show that SEPNET achieves higher detection rates and skill scores while being suitable for real-time space weather alert operations.

How to cite: Chen, Y., Yu, Y., Zhao, L., Whitman, K., Manchester, W., and Gombosi, T.: SEPNET: a multi-task deep learning framework for SEP forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11945, https://doi.org/10.5194/egusphere-egu26-11945, 2026.

EGU26-13611 | ECS | Posters virtual | VPS22

Evaluating the combined potential of VSWIR and Thermal Infrared data for soil characterisation. 

Francesco Rossi, Raffaele Casa, Luca Marrone, Saham Mirzaei, Simone Pascucci, and Stefano Pignatti

Quantifying soil properties such as Soil Organic Carbon (SOC), texture, and Calcium Carbonate (CaCO3) is essential for assessing soil health and ensuring food security. While Visible, Near Infrared, and Short Wave Infrared (VSWIR) remote sensing is a standard operational tool, the Longwave Infrared (LWIR, 8-14 μm) offer complementary information on mineralogy and moisture that are still not yet fully explored for this specific application. This study investigates the synergy between VSWIR and LWIR data that will be available with future hyperspectral satellite missions. Among them, the European Space Agency's Copernicus Expansion missions that will add to the EO capacity the Hyperspectral Imaging Mission for the Environment (CHIME) and Land Surface Temperature Monitoring (LSTM) mission. Alongside are the NASA's Surface Biology and Geology (SBG and SBG-TIR) missions.

The research focuses on Jolanda di Savoia (Italy), an agricultural landscape resulting from land reclamation projects in the late 19th century. Ground truth data were collected during a field campaign on June 22, 2023, providing 59 topsoil samples further analysed for SOC, texture, and CaCO3. Field campaign was coincident with an airborne survey carried out with the LWIR Hyperspectral Thermal Emission Spectrometer (HyTES) sensor. HyTES captured data across 256 spectral bands from 7.5 to 11.5 μm, providing a pixel size of approximately 2.3 meters.

To evaluate the multi-frequency potential, we developed a workflow combining a soil composite from PRISMA (VSWIR) satellite time-series with simulated SBG-TIR (LWIR) data. The SBG-TIR simulation chain included as input a surface emissivity map derived from the airborne HyTES survey. To cover the LWIR wide spectral range (up to 12 µm), the emissivity spectrum was extended using an autoencoder neural network procedure trained on the ECOSTRESS Soil Spectral Library. Top-Of-Atmosphere (TOA) radiance was then simulated using the Radiative Transfer for the TIROS Operational Vertical Sounder (RTTOV-14) model, incorporating the optical depth and cloud/aerosol optical properties coefficients specific to SBG-TIR. Furthermore, these simulated data were atmospherically corrected to produce the target satellite emissivity products according to the TES algorithm.

Soil properties prediction models were developed using supervised machine learning algorithms. We benchmarked two scenarios: 1) the proposed combined approach using PRISMA and the simulated SBG-TIR L2 emissivity product; and 2) a VSWIR-only approach using PRISMA. A quantitative assessment by 10-fold cross-validation using common literature metrics (R², RMSE, RPD) highlighted the benefits of the multi-sensor approach. For SOC retrieval, the standalone VSWIR (PRISMA) model yielded an R2 of 0.55 (RPD = 1.5), while the synergistic integration of PRISMA with simulated SBG-TIR data improved the retrieval accuracy, reaching an R2 of 0.65 and increasing the RPD to 1.69. This work indicates that, on the agricultural test site of Jolanda di Savoia, the combined use of SVWIR and LWIR spectral range slightly improves the SOC retrieval. Further validation across diverse agricultural scenarios will be essential to test the real advantage of combining next-generation imaging spectroscopy missions.

How to cite: Rossi, F., Casa, R., Marrone, L., Mirzaei, S., Pascucci, S., and Pignatti, S.: Evaluating the combined potential of VSWIR and Thermal Infrared data for soil characterisation., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13611, https://doi.org/10.5194/egusphere-egu26-13611, 2026.

Accurate high resolution wind field prediction is essential for wind resource as-
sessment, renewable energy planning, and regional weather analysis. Although
Numerical Weather Prediction (NWP) models such as the Weather Research
and Forecasting (WRF) model provide physically consistent wind forecasts, their
outputs often suffer from systematic biases arising from uncertainties in surface
characteristics, simplified physical parameterizations, and resolution limitations.
Furthermore, increasing model resolution to the kilometer scale significantly
raises computational cost. To address these challenges, this study presents a
machine learning–based framework for bias correction of WRF-simulated wind
fields over the Southern Tamil Nadu region, with particular focus on the Mup-
pandal wind farm area.
An extensive validation of WRF configurations was first performed using mul-
tiple physics scheme combinations and domain setups, evaluated against ERA5
reanalysis data. The optimal configuration was identified and used to gener-
ate three years (2023–2025) of wind simulations at 3 km × 3 km resolution.
Significant biases were observed in the raw WRF outputs, motivating the appli-
cation of an Artificial Neural Network (ANN) based bias correction approach.
A Random Forest algorithm was employed for feature selection, followed by
Principal Component Analysis (PCA) to reduce dimensionality while retaining
95% of the variance. A feedforward neural network with multiple hidden layers
was trained to correct the U10 and V10 wind components, with the hyperbolic
tangent activation function yielding the best performance. The bias-corrected
wind fields exhibited substantial improvement in mean and extremes, achieving low error metrics and
strong correlation with ERA5 data.
The results demonstrate that combining physically based NWP simulations with
machine learning driven bias correction provides an accurate and computation-
ally efficient approach for generating high-resolution wind fields. This hybrid
framework offers significant potential for wind energy assessment and localized
meteorological applications in data-sparse regions.

How to cite: Pm, V. and Chakravarthy, B.: Bias Correction of Numerical Weather PredictionWind Fields in Southern Tamil Nadu RegionUsing Machine Learning Techniques, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16232, https://doi.org/10.5194/egusphere-egu26-16232, 2026.

EGU26-4129 | ECS | Posters virtual | VPS23

Rapid Turbulence Evolution Resulting from Stable Shear layer and Atmospheric Gravity Wave Interactions 

Abhiram Doddi, David Fritts, and Thomas Lund

Early laboratory experiments of shear flow by Thorpe (Thorpe, 2002) provided evidence of Kelvin-Helmholtz Instability (KHI) billow interactions either due to misaligned adjacent billow cores or varying phases along the adjacent billow axes. Similar evidence has been found in the observations of tropospheric clouds, airglow, and Polar Mesospheric Clouds (PMC) imagery data in the mesosphere. Initial High-Resolution Direct Numerical Simulations (DNS) studies performed at Reynolds Number of 5000 (Fritts et al., 2021a, Fritts et al., 2021b) have demonstrated the that misaligned KH billow cores exhibit strong and complex vortex interactions inducing ‘Tubes and Knots’ (T&K) structures (Thorpe, 2002). These T&K structures were observed to accelerate transition to small-scale turbulence in contrast to previously known notable transitional mechanisms such as secondary KHI and convective instabilities emerging in individual KH billows. Also, the KHI T&K dynamics evidently yield intense turbulence dissipation rates contrasting that of secondary KHI and convective instabilities in billow cores.

More recent high-resolution imaging of OH airglow (Hecht et al., 2021) provide concrete evidence of KHI billows with wavelength ranging between 7-10 km modulated by atmospheric Gravity Waves (GWs) of dominant horizontal wavelengths ∼ 30km and oriented orthogonal to KH billow axes and propagate along the billow cores which result in apparent T&K dynamics rapidly driving KH billow breakdown. Similar evidence has been found in recent PMC imaging. This is the central theme of the idealized DNS discussed in this talk.

We conducted DNS studies to demonstrate the turbulence energetics of KHI billow interactions when subject to modulations due to monochromatic atmospheric gravity waves of small perturbation amplitudes and intrinsic frequency of N/5 (where N is the background Brunt-Vaisala Frequency). Preliminary analyses of our DNS results indicate that GW modes with modest amplitudes promote KHI billow misalignments resulting in complex multi-scale T&K dynamics fixed at specific GW phases. An increase in the GW amplitude resulted in noticeable reduction of KHI billow wavelengths further promoting KH billow misalignments. The resulting turbulence is expected to consist of broader scale ranges of intense turbulence dissipation rate and diffusivity.

References
[Fritts et al., 2021a] Fritts, D. C., Wang, L., Lund, T. S., and Thorpe, S. A. (2021a). Multi-Scale Dynamics of Kelvin-Helmholtz Instabilities . Part 1 : Secondary Instabilities and the Dynamics of Tubes and Knots. pages 1–27.

[Fritts et al., 2021b] Fritts, D. C., Wang, L., Thorpe, S. A., and Lund, T. S. (2021b). Multi-Scale Dynamics of Kelvin-Helmholtz Instabilities . Part 2 : Energy Dissipation Rates , Evolutions , and Statistics. pages 1–39.

[Hecht et al., 2021] Hecht, J. H., Fritts, D. C., Gelinas, L. J., Rudy, R. J., Walterscheid, R. L., and Liu, A. Z. (2021). Kelvin-Helmholtz Billow Interactions and Instabilities in the Mesosphere Over the Andes Lidar Observatory: 1. Observations. Journal of Geophysical Research: Atmospheres, 126(1):e2020JD033414. Publisher: John Wiley & Sons, Ltd.

[Thorpe, 2002] Thorpe, S. A. (2002). The axial coherence of Kelvin–Helmholtz billows. Quarterly Journal of the Royal Meteorological Society, 128(583):1529–1542. Publisher: John Wiley & Sons, Ltd.

How to cite: Doddi, A., Fritts, D., and Lund, T.: Rapid Turbulence Evolution Resulting from Stable Shear layer and Atmospheric Gravity Wave Interactions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4129, https://doi.org/10.5194/egusphere-egu26-4129, 2026.

EGU26-4184 | ECS | Posters virtual | VPS23

A Multi-Criteria GIS Framework for Socio-Economic Drought Risk Assessment across India 

Arun kumar Beerkur and Hussain Palagiri

Socio-economic drought represents the stage at which water stress translates into tangible disruptions to livelihoods, infrastructure, and economic systems, often preceding severe physical water shortages. In India, pronounced climatic variability combined with extreme physiographic heterogeneity leads to strong spatial contrasts in socio-economic vulnerability to drought. Despite this, most drought assessments in the country remain dominated by hydro-meteorological indicators, with limited integration of socio-economic exposure, sensitivity, and adaptive capacity.
This study develops a spatially explicit socio-economic drought risk assessment framework for India by integrating multi-dimensional climatic, environmental, and socio-economic indicators within a Geographic Information System (GIS). Thirteen indicators capturing water availability, agricultural productivity, infrastructure, population pressure, economic activity, and social deprivation are compiled from multi-source datasets and harmonized to a common spatial resolution. The indicators include available soil water, agricultural yield, livestock density, road density, population density, biomass, electricity consumption, Gross Domestic Product (GDP), global surface water availability, digital elevation model, groundwater availability, land use/land cover, and relative deprivation. Indicator weights are objectively derived using the Analytic Hierarchy Process (AHP), with consistency of expert judgments ensured through the consistency ratio criterion (CR < 0.1). A GIS-based weighted overlay approach is then employed to generate a composite socio-economic drought risk index, which is classified into four risk categories to identify spatial patterns and hotspots.
The resulting risk map reveals pronounced regional disparities, highlighting drought-prone agrarian and socio-economically marginalized regions as areas of elevated risk. The proposed framework offers a transferable and scalable decision-support tool for integrating socio-economic dimensions into drought monitoring and preparedness. By explicitly linking water stress to livelihood and infrastructure vulnerability, the study provides actionable insights for risk-informed planning, targeted mitigation, and long-term drought resilience in India.

How to cite: Beerkur, A. K. and Palagiri, H.: A Multi-Criteria GIS Framework for Socio-Economic Drought Risk Assessment across India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4184, https://doi.org/10.5194/egusphere-egu26-4184, 2026.

EGU26-4200 | ECS | Posters virtual | VPS23

Performance of Tapered Submerged Vanes in Mitigating Local Scour Around Bridge Piers 

Karmishtha Karmishtha, Rajesh Kumar Behera, and Gopal Das Singhal

Scour, defined as the erosion or removal of sediment from around bridge piers due to flowing water, remains one of the primary causes of hydraulic structure failures worldwide. Local scour around bridge piers poses a serious threat to bridge stability, particularly during high-flow events, as the development of downflow, horseshoe vortices, and wake vortices at the pier base leads to intense sediment removal and foundation instability. To address this challenge, the present study investigates the hydrodynamic behaviour and scour reduction performance of tapered submerged vanes installed upstream of a cylindrical bridge pier as an effective countermeasure against local scour. A combined numerical and experimental approach was adopted to evaluate the influence of tapered submerged vanes on flow structure and scour characteristics. Numerical simulations were carried out using FLOW-3D Hydro to analyse the three-dimensional flow field around the pier–vane system under steady clear-water conditions. The simulations focused on assessing velocity distribution, near-bed shear stress, vortex dynamics, and secondary flow patterns generated by the tapered vanes. Particular attention was given to the formation of leading-edge vortices (LEVs) and their role in modifying erosive flow structures near the pier foundation. Based on the numerical insights, a series of physical model experiments were conducted in a laboratory flume to quantify the scour reduction achieved by the tapered vanes. The experiments aimed to optimize the longitudinal and transverse placement of the vanes relative to the pier. The vanes were installed at a fixed longitudinal distance upstream of the pier, while transverse spacing was systematically varied to examine its effect on sediment transport and scour depth. Bed elevation profiles and maximum scour depths were measured after equilibrium scour conditions were attained. The results demonstrate that tapered submerged vanes significantly alter the near-bed flow field by generating localized leading-edge vortices that effectively deflect high-energy flow away from the pier base. This flow redirection weakens the horseshoe vortex and reduces near-bed shear stress in the vicinity of the pier. Among the tested configurations, the vane arrangement with a longitudinal spacing of 1.5D and transverse spacing of 2D exhibited the best performance, resulting in a 56% reduction in maximum scour depth compared to the no-vane case. Additionally, localized sediment deposition was observed upstream and downstream of the pier, indicating favourable redistribution of sediment induced by the vane-generated secondary currents. By integrating numerical modelling with experimental validation, this study provides valuable insights into the flow mechanisms and optimal placement strategies of tapered submerged vanes. The findings highlight their potential as a practical, efficient, and sustainable solution for mitigating local scour around bridge piers in alluvial channels.

Keywords: Scour, Submerged Vane, Horseshoe Vortices, Wake Vortices, Leading-Edge Vortex (LEV)

How to cite: Karmishtha, K., Behera, R. K., and Singhal, G. D.: Performance of Tapered Submerged Vanes in Mitigating Local Scour Around Bridge Piers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4200, https://doi.org/10.5194/egusphere-egu26-4200, 2026.

EGU26-4951 | ECS | Posters virtual | VPS23

CFD-Based Comparative Analysis of Conventional and Modified Piano Key Weirs for Improved Discharge Efficiency 

Anil Kumar, Ellora Padhi, and Surendra Kumar Mishra

The Piano Key Weir (PKW) has earned recognition for its adaptability for large discharges across weir types of varying heights and with small footprints. Therefore, it has the potential to be a substitute for linear weirs (space being a factor), Ouamane and Lempérière, (2006). Even with the above-mentioned advantages of PKWs, other geometries leave much to be desired. The rectangular PKW and the trapezoidal PKW illustrate a most common inefficiency example. Standard literature describes construction and operational shortfalls such as flowing separation at the inlet key, varying discharge and uneven velocities along the crest, vortex shedding and formation at the key intersections, dead zones in the inlet-outlet, zones of intensified energy dissipation, and lowering weir versatility at high flows. These challenges are combined to mean loss of efficiency in weir discharge capability. In response to these challenges, the present study introduces the Modified Piano Key Weir (MPKW) to assess its performance using 3D computational hydraulic modeling. The Volume of Fluid (VOF) methodology for free surface tracking and the Reynolds-Averaged Navier Stokes (RANS) for turbulence closure modeling characterize pressure gradients, flow accelerations in the several dimensions, and eddies. A systematic numerical investigation was conducted to compare the discharge efficiency of RPKW, TPKW, and MPKW across a range of steady inflow discharges: 0.030, 0.060, 0.090, 0.120, and 0.160 m³·s⁻¹. The MPKW demonstrated consistently superior discharge efficiency over both RPKW and TPKW for all tested cases, without requiring an increase in structural footprint or crest length. The highest relative improvement was observed at 0.060 m³·s⁻¹, which was therefore selected as a representative discharge for in-depth flow diagnostics. Discharge at 0.060 m³·s⁻¹ was applied to determine vorticity structures, turbulent kinetic energy (TKE), and energy dissipation to better understand the flow mechanisms that explain the efficiency of the weir. The MPKW design, with refined geometry and improved inlet–outlet design, rounded key transitions, and adjustable wall skew, was successful in mitigating flow separation at the key inlets and reducing the large-scale vortex formation at the key junctions. The modified sidewall skewed the internal recirculation, and as a consequence, TKE in the stagnation zones was less, and recirculation was more along the crests of the weir, thereby nullifying turbulent structures. While the breakdown of turbulence resulted in localized energy dissipation, the stabilization of the approach flow was improved because the process converted rotational energy of large eddies with a low energy loss to rapidly decaying eddies which do not sustain and produce a recycling of energy. Thus, less energy was concentrated in the vortex cells at the key junctions, the loss due to flow contraction was less, and the nappe cohesion over the crests was improved. MPKW, relative to other configurations, was characterized by a lower level of turbulence and vorticity at the junctions, a greater effective utilization of the crest, and improved pressure recovery. The results confirm MPKW as a hydraulically efficient and economically feasible solution for both new installations and retrofit applications under head or footprint constraints.

How to cite: Kumar, A., Padhi, E., and Mishra, S. K.: CFD-Based Comparative Analysis of Conventional and Modified Piano Key Weirs for Improved Discharge Efficiency, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4951, https://doi.org/10.5194/egusphere-egu26-4951, 2026.

EGU26-5098 | ECS | Posters virtual | VPS23

A Geospatial and AHP-Based Approach for Delineating Groundwater Potential Zones in Vulnerable Groundwater Systems 

Pavithra Belluti Nanjundagowda and Vamsi Krishna Vema

Groundwater is the second largest reserve of fresh water and is an important resource that supports agriculture, industrial and domestic water supplies. Groundwater is facing unsustainable impacts by human activities over the years in different forms. The situation is aggravated by climate change which aggravates groundwater stress through variable precipitation leading to reduced recharge. Thus, highlighting the importance of assessing aquifer potential for sustainable groundwater management. The analysis was carried out in the Manjra and Maner sub-basins, of Godavari river basin, India where data-driven assessments remain limited. In this regard, the present research employs a Multi-Criteria Decision Analysis (MCDA) framework that integrates Geographic Information Systems (GIS) and the Analytical Hierarchy Process (AHP) to define groundwater potential zones (GWPZ) in the Manjra and Maner sub-basins. In a GIS environment, eight thematic layers—geology, land use/land cover, lineament density, drainage density, rainfall, soil, and slope—were examined. These factors were weighted using AHP, and combined using weighted overlay analysis. Area under the Curve (AUC), Receiver Operating Characteristic (ROC) analysis, and groundwater inventory data were used to validate the final GWPZ map. Five classifications of groundwater potential were identified for the research area: very low, low, moderate, high, and very high. The research region's predominance of moderate (45%) to high potential (28%) zones suggests that groundwater availability is generally fair to good. Priority locations for sustainable groundwater development and management are indicated by the high and very high potential zones.

How to cite: Belluti Nanjundagowda, P. and Vema, V. K.: A Geospatial and AHP-Based Approach for Delineating Groundwater Potential Zones in Vulnerable Groundwater Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5098, https://doi.org/10.5194/egusphere-egu26-5098, 2026.

EGU26-5765 | ECS | Posters virtual | VPS23

Research on the mechanical behaviors of multi-fractured blocky rock masses 

Kuan Jiang, Chengzhi Qi, and Xiaoyue Hu

Deep rock masses have complex internal structures, which results in significant discreteness and blocky structures. With the increase in the depth of engineering construction and energy extraction, the unique pendulum-type waves emerge in deep blocky rock masses under the action of dynamic loads from mining and blasting, and they are characterized by low frequency, low velocity, large displacement amplitude and high kinetic energy, distinguishing them fundamentally from conventional seismic waves. Pendulum-type waves can induce alternating stress states of relative compression and separation within blocky rock masses, and may lead to rockburst disasters and even engineering-induced seismicity, thus posing great challenges to the safety of underground engineering such as tunnel construction and mining. In this paper, experimental research is conducted on the mechanical behaviors and typical characteristics of pendulum-type waves of multi-fractured blocky rock masses under static and dynamic loads. Firstly, the strength, deformation and failure mode were analysized based on uniaxial compression tests. The weak structural layers will significantly reduce the uniaxial compressive strength and enhance the ultimate deformation capacity of rock masses. Fractured rock masses have significant nonlinear deformation and may develop macroscopic fractures (vertical splitting failure, with the failure mode transitioning from brittle failure to ductile failure) at the stress level significantly lower than their uniaxial compressive strengths. Subsequently, based on the dynamic impact tests, the dynamic response, overall displacement, wave velocity and the mechanism of anomalously low friction were investigated, and the typical characteristics of pendulum-type waves, including the low frequency (177 Hz and 153 Hz in this experiment, which are much lower than the natural frequency of the rock itself), low velocity (about 900 m/s in this experiment, which is significantly lower than those of P-waves and S-waves), large displacement amplitude (it is more than two orders of magnitude larger than the deformation of an intact rock under an identical load) and high kinetic energy (The total kinetic energy accounts for 40% and 28% of the total energy in this experiment, which has its particularity and cannot be ignored) were quantitatively described. This study holds significant research importance for understanding the nonlinear waves in deep fractured rock masses and their dynamic behaviors, as well as for preventing and controlling engineering disasters in deep rock masses.

How to cite: Jiang, K., Qi, C., and Hu, X.: Research on the mechanical behaviors of multi-fractured blocky rock masses, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5765, https://doi.org/10.5194/egusphere-egu26-5765, 2026.

Predictability of river bank erosion in sinuous alluvial channels requires a combined study of the planform processes, hydraulics processes, sediment transportation, and the geotechnical properties of riverbanks. The research paper provides a detailed analysis of the evolution of channels within the Nabadwip-Kalna stretch of the Bhagirathi-Hooghly River (1990-2020). This analysis combines the synthesis of remote sensing, on-field surveys, lab experiments, and numerical model analysis into a multidimensional analysis. GIS was used through the Digital Shoreline Analysis System (DSAS) to measure changes on the bank-lines using historical satellite images of the same period of time. A two-dimensional migration coefficient (MC) model was used to model spatial-temporal changes in channel centrelines, and an RVR Meander was used to develop a model that takes into consideration depth-averaged flow velocity and reach-averaged hydraulic parameters. The characterisation of cross-sectional bathymetry and near-bank hydraulics was based on ADCP. The results of the geotechnical analysis showed that stratified streambanks showed critical shear stresses of 7.1-7.7 kPa, internal frictional angles of soils less than 30°–34°, and were predominantly affected by either cantilever collapse or piping as a result of varying maximum heights of streams between 5.7 and 6.8 metres. Bank stability through both BSTEM and BEHI was assessed, whereas sediment forecasting combined with SWAT to predict overbank flow and a Genetic Algorithm (GA) to estimate the total load. DSAS analysis on bank-line displacement revealed different erosion patterns within 170 transects, showing different RMSE of 0.090 to 0.162 in predicting zone boundaries. The MC method was able to model the 24-year centreline migration patterns, recording changes in the centreline-geometry parameters. Analysis of five cross-sections instrumented found instability and a factor-of-safety ratio of 0.81-0.95, resulting in 4.07-5.85m/yr and 4.35-7.15 km2/yr, respectively, lateral retreat and the eroded areas. Mean collapse rates were 0.125 to 0.198 m/yr, and the failure angle was 81°–87°. The maximum bank-failure mass was 41.24 kg (seasonal maximum), and the calibrated toe-scour mass was 0.28 kg. The GA model was tried using ten parameterisations and demonstrated the best prediction ability with the coefficient set at ten, where R2 = 0.96 and mean relative error (MRE) = 42% gave significantly better performance than the traditional regression analysis (R2 = 0.87 and MRE = 40%). There were also considerable changes in the area behind sandbar dynamics, that is, Nandai-Hatsimla increased by 11.87 ha in 1990 to 19.05 ha in 2020; Media by 39.7 ha to 57.68 ha; Char Krishnabati by 82.52 ha to 81.07 ha. Land-use/land-cover (LULC) predictions for 2040 indicated settlement expansion from 13.61% (2020) to 20.19%, with validation accuracy (RMSE = 0.253) confirming model reliability. This combined model shows that the combination of remotely sensed, field, laboratory, and model data provides quantitatively sound estimations of fluvial risks and forms the basis of evidence-based management of high-suspended riverine areas. The modular design can be applied to monsoon-dominated alluvial basins throughout the globe, which will promote adaptive land-use planning and long-term infrastructure development in the vulnerable riparian societies.

How to cite: Ghosh, A.: Unveiling integrated geo-hydraulic assessment of river meandering, bank erosion and sandbar dynamics in Alluvial channels, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7917, https://doi.org/10.5194/egusphere-egu26-7917, 2026.

EGU26-8596 | ECS | Posters virtual | VPS23

Waveform signatures of acoustic emission from thermally and mechanically induced microfracture in centrally apertured basalt 

Arthur De Alwis, Mehdi Serati, Arcady Dyskin, Elena Pasternak, Derek Martin, and David Williams

Acoustic emission (AE) monitoring is widely applied to track damage development in brittle rock, although relating recorded signals to specific fracture mechanisms can remain uncertain, particularly when comparing thermal and mechanical loadings. This contribution presents a preliminary assessment of AE waveform characteristics measured during two heating-only experiments and two uniaxial compressive strength (UCS) experiments performed on 100 mm diameter basalt specimens containing a central axial circular hole. This geometry provides a consistent configuration that promotes stress redistribution and damage localisation around an opening, allowing fracture processes to be compared within a common specimen form.

Full AE waveforms were acquired throughout each test using broadband piezoelectric sensors coupled to the specimen surface, with pre-amplification and digital acquisition. Event features were extracted in the time and frequency domains, including rise angle, duration, hit counts, average frequency, peak frequency, peak amplitude, and amplitude distributions. Feature-space comparisons were then used to evaluate whether thermally and mechanically induced microfracturing exhibit separable signal characteristics.

The thermal experiments were associated with a single dominant fracture initiating along the shortest ligament between the aperture boundary and the nearest specimen edge. In contrast, UCS loading produced a more complex fracture network consistent with mixed tensile and shear microfracturing. Rise angle versus hits per duration plots indicated that thermal events occupied a more restricted region, whereas UCS events displayed a broader spread, which may reflect greater variability in source processes during complex damage evolution. Frequency-based comparisons further highlighted the differences: thermally induced events clustered mainly within a lower-frequency band (approximately 100-300 kHz), while the UCS tests exhibited an additional higher-frequency population (approximately 400-600 kHz), alongside the lower-frequency component. Amplitude distributions were also differed, with thermal events tending toward a narrower amplitude range relative to the wider distribution observed under UCS loading. Collectively, these observations suggest that the combined time-domain, frequency-domain, and amplitude-based AE features support mechanism-informed discrimination between thermally driven tensile fracture and mechanically driven complex fracture networks providing a basis for subsequent statistical or learning-based classification in coupled thermomechanical experiments

How to cite: De Alwis, A., Serati, M., Dyskin, A., Pasternak, E., Martin, D., and Williams, D.: Waveform signatures of acoustic emission from thermally and mechanically induced microfracture in centrally apertured basalt, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8596, https://doi.org/10.5194/egusphere-egu26-8596, 2026.

EGU26-8813 | ECS | Posters virtual | VPS23

Assessment of Partial Blockage in Urban Drains for Flood Risk Reduction  

Aayusha Kumari Mishra, Hemant Kumar, and Rajendran Vinnarasi

Partial blockage in open channels and urban drainage systems is a common issue arising from debris accumulation, sediment deposition, and inadequate maintenance, often resulting in reduced flow capacity and increased flood risk. Despite its practical relevance, the hydraulic effects of partial blockage on flow behaviour are not well quantified through controlled experimental studies. This work aims to investigate the influence of partial blockage on flow characteristics in open channels and explore its implications for urban stormwater drainage systems.Laboratory experiments are carried out in a rectangular open-channel flume under steady flow conditions. Velocity measurements are obtained at multiple depths for unblocked conditions and for different partial blockage configurations. Blockages of varying size and location are introduced manually to represent realistic obstructions commonly observed in urban drains. The changes in velocity distribution, water depth, and flow-carrying capacity due to partial blockage are analysed to understand the hydraulic response of the system.

Based on these observations, relationships between blockage extent and hydraulic performance are developed to identify critical blockage conditions.The study framework is applied to urban stormwater drainage networks using SWMM modelling to extend the experimental findings to real-world applications. Blockage scenarios are simulated in selected channels to assess their impact on system performance and flooding behaviour.

The outcomes of this study provide experimental insight into blockage-induced hydraulic effects and highlight the importance of considering partial blockage in urban drainage analysis. The combined experimental and modelling approach offers a practical basis for improving flood risk assessment and maintenance planning in urban stormwater systems.

How to cite: Mishra, A. K., Kumar, H., and Vinnarasi, R.: Assessment of Partial Blockage in Urban Drains for Flood Risk Reduction , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8813, https://doi.org/10.5194/egusphere-egu26-8813, 2026.

Rising flooding, which is exacerbated by both climate change and human behavior, demands proper identification of vulnerable zones. Conventional hydrological analysis can neglect geographical variability. In this study, a combined geospatial and decision-making process is used to determine the levels of vulnerability and risk of flooding in the Koshi River Basin in the state of Bihar.  The research work has developed a susceptible, vulnerable and risk map by integrating GIS, Remote Sensing and AHP. Weightings of eleven physical and hydrological factors and five socio-economic indicators were carried out in a systematic manner using a multi-criteria decision-making framework that allowed appropriate consideration of their relative contributions to flooding. Flood susceptibility, vulnerability and risk maps were created using the GIS environment's Weighted Overlay technique. According to the analysis, population density (41.6%) and literacy rate (24%) are controlling factors for flood vulnerability in the basin, whereas rainfall (23.9%), elevation (14.7%) and drainage density are the main elements that influence flood susceptibility. The Koshi basin is largely covered by the low and moderate classes of flood susceptibility, whereas a very minor amount (0.03%) comes under the high susceptibility classes, according to results from flood susceptibility maps. A significant section (42.87%) of the basin has moderate flood susceptibility due to a combination of exposure and socioeconomic characteristics, according to the results of the flood vulnerability analysis. According to the flood risk results, a significant amount of the basin (84.18%) has moderate flood risk, while a tiny portion has high flood risk in the low-lying, heavily inhabited areas close to the basin's riverbanks.  ROC-AUC for model validation yielded an accuracy of 66.3% and proved that the proposed GIS-AHP model was a reliable. Conclusion from this study underscore an integrating role in both physical and socio-economic considerations with prospects of enhancement through climate scenarios in flood mitigation and planning/early warning maps.

How to cite: Chaudhary, P. and Padhi, E.: Flood Hazard Analysis and Risk Assessment of Koshi River, Bihar (India) using Remote Sensing, GIS and AHP Techniques , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8975, https://doi.org/10.5194/egusphere-egu26-8975, 2026.

EGU26-8985 | ECS | Posters virtual | VPS23

Non-linear rotational waves and complex rotation patterns in a chain of blocks with elbowing 

Maoqian Zhang, Arcady Dyskin, and Elena Pasternak

Block elbowing, the process in which rotating blocks push neighbouring blocks apart, influences both geological deformation and the stability of mining excavations in blocky rock masses. A clearer understanding of elbowing is essential for improving rock mass modelling and maintaining the safety of engineering structures. To this end, we analyse a chain of stiff blocks connected by springs, with one or two end active (driving) blocks – the blocks whose rotation is externally induced. All other - passive blocks - have translational and rotational degrees of freedom. The results show that block rotation is sequential (starting from driving blocks) producing a rotational wave with strongly configuration-dependent rotational patterns.

Opposite to a single driving block system, a double-driving block system exhibits more complex behaviour, as the active blocks may rotate in the same direction (Case I) or in opposite directions (Case II). In Case I passive blocks can exhibit anticlockwise rotation that is opposite to the clockwise rotating driving blocks, while in Case II all passive blocks do not rotate at all.

Further deformation patterns arise from block geometry, introduced by varying block corner rounding to represent spheroidal weathering. The results reveal a transition from reversible to irreversible passive block kinematics. Reversible responses include either clockwise rotation followed by full recovery or no rotation. The boundary between these types of block behaviour is defined by a linear relationship between the active-passive and passive-passive contact friction coefficients, with the intercept related to block corner rounding. In contrast, irreversible kinematics characterised by residual rotation emerge only for highly rounded blocks. This irreversible behaviour is restricted to short block chains and disappears in chains of five blocks suggesting a critical size of the Cosserat like zone with independent rotational degrees of freedom. This study provides new insights for modelling the stability and long-term evolution of blocky rock masses.

How to cite: Zhang, M., Dyskin, A., and Pasternak, E.: Non-linear rotational waves and complex rotation patterns in a chain of blocks with elbowing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8985, https://doi.org/10.5194/egusphere-egu26-8985, 2026.

The subject of this study is the process of hydraulic stimulation of a tectonic fault, leading to induced seismicity. We consider a scenario in which fluid injected near ​​an existing fault, causing a localized change in pore pressure and a reduction in effective stresses. This, in turn, initiates slippage of the fault segments and the formation of a slip zone, the size and slip velocity of which determine the magnitude of the resulting seismic events. The goal of this study was to develop a relatively simple model for estimating the potential magnitude of induced seismic events based on a limited set of governing parameters. The primary objectives of the study were to identify the key factors that have the greatest impact on the characteristics of the slip zone and to determine how fluid injection parameters (rate and injected fluid volume) affect earthquake magnitude by changing slip dynamics. The model obtained is based on the results of a series of numerical experiments analyzing the hydromechanical behavior of the fault under various injection conditions. The modeling was performed using a two-parameter rate-and-state friction law, which, unlike a single-parameter model, allows for a wider range of slip regimes to be simulated and accurately describes the transition from stable slip to dynamic failure.

The functional relationships were established between the initial system parameters and the key obtained slip characteristics. It was shown that the final slip zone length is almost linearly related to the length of the initial unstable zone, and the maximum slip velocity increases exponentially with increasing pore pressure rate. At the same time, in the area of high loading rates, the saturation of the sliding velocity is observed at a characteristic level, which leads to a limitation of the possible magnitudes of earthquakes induced by fluid injection.

How to cite: Turuntaev, S., Baryshnikov, N., and Riga, V.: Estimation of potential magnitudes of induced seismic events based on direct numerical simulation of fluid injection near an active tectonic fault., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11339, https://doi.org/10.5194/egusphere-egu26-11339, 2026.

EGU26-13831 | ECS | Posters virtual | VPS23

From Empirical Assumptions to Data-Informed Decisions: A Reliable Water Storage Soil Depth Estimation Method 

Damodar Sharma, Surendra Kumar Mishra, and Rajendra Prasad Pandey

Efficient water use in agriculture is crucial for sustainable water resource management, especially in areas experiencing increasing water scarcity. A critical yet often oversimplified component of irrigation planning is the estimation of water storage soil profile depth, commonly assumed to be 1-1.5 m as the root-zone depth based on practitioner experience rather than validated soil-water dynamics. Such assumptions introduce uncertainty and limit the reliability of irrigation scheduling decisions. This study presents a novel framework for estimating soil profile depth to store maximum water by integrating Richards’ equation, geotechnical soil column concepts, and the Soil Conservation Service Curve Number (SCS-CN) technique to derive an optimal soil profile depth that maximizes storage capacity based on measurable hydraulic and retention soil properties. By linking the water storage soil column depth with the SCS-CN parameter, for practical field applications such as irrigation scheduling and planning. The proposed framework improves model reliability and interpretability by replacing fixed-depth assumptions with soil-specific storage behaviour, thereby reducing uncertainty in irrigation water estimation. It enables consistent evaluation of field capacity, average soil moisture content, and maximum storage potential across soil types, leading to improved irrigation efficiency. By emphasizing physically constrained model selection, data-informed parameterization, and transparent decision-making metrics, this work enhances the reliability of hydrologic modeling and supports robust irrigation management under water-scarce conditions.
Keywords:  Water storage soil profile depth, Richards’ equation, Irrigation water management, Data-informed parameterization, SCS-Curve Number method.

How to cite: Sharma, D., Mishra, S. K., and Pandey, R. P.: From Empirical Assumptions to Data-Informed Decisions: A Reliable Water Storage Soil Depth Estimation Method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13831, https://doi.org/10.5194/egusphere-egu26-13831, 2026.

EGU26-15102 | Posters virtual | VPS23

Anisotropic energy transfer rate quantified by LPDE and directional averaging methods in MHD turbulence 

Zhuoran Gao, Yan Yang, Bin Jiang, and Francesco Pecora

The energy cascade rate (ε) depicts the energy transfer in a turbulent system. In incompressible magneto-hydrodynamic (MHD)  turbulence, ε is linked to the third-order structure function (Yaglom vector) via the Yaglom/Politano–Pouquet law in the inertial range. In this study, we compare three estimators of ε in anisotropic MHD turbulence: (1) the lag polyhedral derivative ensemble (LPDE) technique that reconstructs the divergence of the Yaglom vector via tetrahedral linear gradients; (2) a directional-averaged third-order estimator that evaluates the Yaglom vector along a finite number of lag directions and averages over solid angle; and (3) the Yaglom vector on 60 degree with respect to the mean magnetic field direction.  To ensure a fair comparison in more realistic MHD turbulence, we emulate a multipoint virtual mission within anisotropic three-dimensional MHD simulations with a guide field B₀ along the z-axis. This work illuminates the reliable regime for LPDE and directional-averaging methods, and also tests whether 60 degree Yaglom vector is an accurate estimate of ε, providing practical guidance in both simulation and observational turbulence analysis.

How to cite: Gao, Z., Yang, Y., Jiang, B., and Pecora, F.: Anisotropic energy transfer rate quantified by LPDE and directional averaging methods in MHD turbulence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15102, https://doi.org/10.5194/egusphere-egu26-15102, 2026.

EGU26-16403 | ECS | Posters virtual | VPS23

Assessing the Impact of Digital Elevation Model Selection on Hydrological Predictions 

Prashant Prashant, Surendra Kumar Mishra, and Anil Kumar Lohani

Digital elevation models (DEMs) play a fundamental role in hydrological modeling by controlling watershed delineation, stream networks and runoff generation processes. This study assess the impact of global DEM product provided by Shuttle Radar Topography Mission SRTM and the Indian national CartoDEM developed by ISRO-Bhuvan (Indian Space Research Organisation-Bhuvan) on streamflow simulation using the Soil and Water Assessment Tool (SWAT) in the Ong River watershed (4650 sq. km), India. The study area is characterized by forest and cropland. Both DEMs, resampled to 30m resolution, were used as inputs to SWAT, along with meteorological data (IMD), land use/land cover data (Sentinel-2), and soil data (FAO). Streamflow data was sourced from Global Flood Awareness System discharge data (GloFAS). Model calibration (2011-2017) and validation (2018-2020) were performed using SWAT-CUP with the SUFI2 algorithm. Model performance was evaluated using Willmott's index of agreement, Nash-Sutcliffe Efficiency (NSE), R², PBIAS, and RSR. Results showed that both DEMs performed satisfactorily, with CartoDEM exhibiting slightly better performance (higher NSE and R², lower PBIAS and RSR) during both calibration and validation periods. Sensitivity analysis revealed that the runoff curve number was the most sensitive parameter, highlighting the impact of DEM selection on surface runoff simulation. The study concluded that CartoDEM is a preferable choice for hydrological modeling in similar catchments, though further research on stream accuracy and catchment delineation in diverse topographies can be explored.

How to cite: Prashant, P., Kumar Mishra, S., and Kumar Lohani, A.: Assessing the Impact of Digital Elevation Model Selection on Hydrological Predictions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16403, https://doi.org/10.5194/egusphere-egu26-16403, 2026.

EGU26-18007 | ECS | Posters virtual | VPS23

Effects of Flow Depth and Sediment Size on Near Bed Hydraulics and Sediment Mobility in Open Channel Flow 

Jyothi Banothu and Kamalini Devi

Accurate prediction of sediment mobility in open channel flows is essential for effective river engineering and sediment management. This study examines the combined influence of flow depth and sediment grain size on near bed hydraulics and sediment mobility using high-resolution Acoustic Doppler Velocimeter (ADV) measurements in a controlled laboratory flume. Experiments were conducted over uniform sand beds with median grain sizes of d₅₀ = 0.321 mm and d₅₀ = 0.81 mm under four different flow depths (12cm, 15cm,18cm,21cm) and a range of flow velocities. Three dimensional velocity components were measured at multiple vertical locations throughout the flow depth, while water surface elevations were continuously monitored. Depth resolved ADV data were used to compute mean streamwise velocity, Reynolds shear stress, friction velocity, and turbulent kinetic energy for each sediment size and flow depth. Sediment mobility was assessed using the Shields parameter, estimated from ADV-derived bed shear stress, and compared with the critical Shields parameter at multiple velocity points for each depth. The results indicate that coarser sediment beds exhibit increased near-bed turbulence intensity and higher friction velocity across all flow depths, while yielding lower Shields parameter values relative to finer sediment beds. Comparisons across the four flow depths reveal that sediment mobility transitions from stable to mobile conditions depending on the combined effects of flow depth, sediment size, and local velocity magnitude. At lower velocities, Shields parameter values remain below the critical threshold, indicating stable bed conditions, whereas higher velocities at the same depth result in Shields values exceeding the critical limit, signifying active sediment motion. Depth wise velocity and turbulence profiles demonstrate that both flow depth and sediment roughness significantly modify near-bed hydraulic structure and bed shear stress distribution. The findings highlight the importance of accounting for depth-dependent flow structure and sediment characteristics when evaluating sediment mobility. This study provides a robust experimental framework for identifying stable and mobile sediment regimes and estimating sediment transport potential using high-resolution ADV measurements without direct sediment transport observations.

How to cite: Banothu, J. and Devi, K.: Effects of Flow Depth and Sediment Size on Near Bed Hydraulics and Sediment Mobility in Open Channel Flow, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18007, https://doi.org/10.5194/egusphere-egu26-18007, 2026.

EGU26-18481 | ECS | Posters virtual | VPS23

Assessing urban surface flood resilience using hydrodynamic modelling under extreme rainfall conditions in urban catchment of Nepal 

Pushparaj Singh, Rahul Deopa, and Mohit Prakash Mohanty

Urban flooding poses a growing challenge for rapidly urbanizing cities, where climate change–driven increases in extreme rainfall, expanding impervious surfaces, and limited drainage capacity collectively exacerbate the frequency and severity of surface water inundation. In this context, understanding urban surface flood resilience, defined as the capacity of stormwater drainage systems to withstand, convey, and recover from intense rainfall events, remains essential for effective flood risk management and climate adaptation planning. The present study investigates urban surface flood resilience in Janakpur Sub-Metropolitan City, Nepal, a fast-growing urban center increasingly exposed to pluvial flooding. The study develops an integrated modelling framework using a 3-way coupled MIKE+ hydrodynamic model, integrated with intense spatial analysis using GIS, to evaluate the performance of the existing stormwater drainage system under extreme rainfall conditions. The model represents the urban drainage network and surface flow processes using drainage infrastructure data obtained from field surveys, terrain information derived from a high-resolution digital elevation model, and delineated urban catchments. To characterize rainfall extremes, the analysis employs long-term observed hourly rainfall records spanning 25 years to generate design storm events corresponding to multiple return periods. The modelling framework simulates system response for a representative extreme rainfall event and quantifies inundation dynamics across the urban landscape. The results shows that the coupled approach effectively captures critical flood hazard characteristics, including inundation depth, flow velocity, and the depth–velocity product, allowing for the spatial identification of highly vulnerable catchments and drainage bottlenecks. The findings provide actionable insights into the limitations of existing stormwater infrastructure and support the development of targeted adaptation strategies aimed at enhancing urban surface flood and drainage resilience. Overall, the study underscores the value of integrated hydrodynamic modelling for resolving location-specific flood behaviour and strengthening urban flood resilience assessments under evolving climatic and urbanization pressures.

How to cite: Singh, P., Deopa, R., and Mohanty, M. P.: Assessing urban surface flood resilience using hydrodynamic modelling under extreme rainfall conditions in urban catchment of Nepal, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18481, https://doi.org/10.5194/egusphere-egu26-18481, 2026.

EGU26-18820 | ECS | Posters virtual | VPS23

Global climate dynamics in a highly parameterized radiative-convective-macroturbulent energy balance model 

Adrian van Kan, Jeffrey Weiss, and Edgar Knobloch

We present a one-layer global energy balance climate model with highly parameterized radiation, convection, and large-scale atmosphere/ocean macroturbulence. Planetary heat content is parameterized by a 2D in latitude-longitude layer characterized by a temperature field and a uniform constant heat capacity. Radiation is parameterized by mean-annual zonal average top-of-atmosphere solar irradiance. Radiative heating and cooling are parameterized by a uniform constant albedo and Stefan-Boltzmann emission with uniform constant emissivity. Convection is parameterized by a temperature threshold for convection which restricts the layer from warming beyond the threshold, effectively cooling the layer. Macroturbulence is parameterized by 2D barotropic turbulence forced at small scales and damped by Rayleigh friction. Energy conservation is maintained by balancing the convective cooling of the layer with the turbulent kinetic energy forcing, resulting in tropical forcing, while the frictional loss of kinetic energy is balanced by frictional heating of the layer. The parameterized energy transforming processes are characterized by timescales, which, for Earth-like planets, are ordered as tradiation > tmacroturbulence > tconvection.

We investigate the model’s equilibrium climate state in terms of the meridional heat transport (MHT), the resulting zonally averaged temperature profile, and their fluctuations by simulating the system over many radiation times. For Earth-like parameters, despite the model’s extremely simplified dynamics, our simulations reveal a MHT profile comparable to the observed, annually averaged MHT on Earth, featuring a maximum in the mid-latitudes of approximately 5PW, a form of Bjerknes compensation. 

How to cite: van Kan, A., Weiss, J., and Knobloch, E.: Global climate dynamics in a highly parameterized radiative-convective-macroturbulent energy balance model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18820, https://doi.org/10.5194/egusphere-egu26-18820, 2026.

EGU26-19471 | ECS | Posters virtual | VPS23

From bilinear interpolation to machine learning: a comparative assessment of statistical downscaling methods for CMIP6 projections over Brazil 

Diego Jatobá Santos, Gilberto Goracci, Minella Alves Martins, and Rochelle Schneider

High-resolution climate projections are essential for climate impact, vulnerability, and adaptation studies, particularly over regions with strong spatial heterogeneity such as Brazil. Although CMIP6 global climate models (GCMs) provide valuable information on future climate change, their coarse spatial resolutions, typically ranging from 100 to 200 km, limit their direct application at regional and local scales. Statistical downscaling techniques offer computationally efficient alternatives to dynamical downscaling, but their relative performance and added value remain insufficiently assessed over Brazil.

In this study, we compare two statistical downscaling approaches applied to a subset of CMIP6 models previously evaluated by Bazanella et al. (2024) – 10.1007/s00382-023-06979-1 – and identified as skillful in representing Brazilian climate: (i) a bilinear interpolation method followed by percentile-to-percentile bias correction, and  (ii) machine learning–based downscaling approaches. The original GCM outputs are interpolated to a common high-resolution grid of 10 km × 10 km using bilinear weights, providing a physically consistent reference framework. In parallel, ML-based models are trained using historical GCM predictors and high-resolution reference climate datasets to learn nonlinear relationships and generate high-resolution climate fields.

The performance of both approaches is evaluated for the historical period in terms of mean climatology, spatial patterns, and variability. Future projections under the SSP2-4.5 and SSP5-8.5 scenarios are then analyzed to assess regional climate change signals and associated uncertainties. Results assess the extent to which ML-based downscaling provides added value relative to bilinear interpolation, particularly for variables with strong spatial heterogeneity, such as precipitation and temperature extremes, while also evaluating the ability of the approach to preserve the large-scale climate signals projected by the driving CMIP6 models. This comparative analysis provides insights into the applicability, robustness, and limitations of statistical and ML-based downscaling methods for regional climate assessments over Brazil.

How to cite: Jatobá Santos, D., Goracci, G., Alves Martins, M., and Schneider, R.: From bilinear interpolation to machine learning: a comparative assessment of statistical downscaling methods for CMIP6 projections over Brazil, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19471, https://doi.org/10.5194/egusphere-egu26-19471, 2026.

Accurate estimation of evapotranspiration (ET) is critical for various applications in hydrology and agricultural water management. However, direct observations of ET, specially its spatial variation, in time-consuming and cumbersome, thus necessitating the need to use of indirect methods for its estimation. In this study, stomatal conductance data is used in conjunction with bio-physical parameters of wheat crops for deriving the spatially varied estimates of ET (ETSC) for different irrigation treatments using the Penman-Monteith equation. For this, five treatments, including drip (DI) and flood (FI) irrigated treatments were used in the study, namely fully irrigated (DI)), 50% MAD (maximum allowable deficit) (DI), 50% MAD (FI), farmer fields replication (FI) and rain-fed treatment.

The ETSC estimates are also compared to the ET estimates derived using a method based on field water balance (ETWB). When compared with the ETWB values, the ETSC estimates compared well particularly for the irrigated treatments. The average root mean square error (RMSE) of ETSC estimates in comparison to ETWB values are 0.11, 0.2, 0.23 and 0.26 mm/day for fully irrigated, 50% MAD (FI), 50% MAD (DI) and farmers field replication treatments, respectively. The corresponding RMSE value (0.47 mm/day) for the rain-fed treatment are found significantly higher than the irrigated treatments indicating the limitation of the approach in high water stress conditions. The differences between ETSC andETWB values also increase significantly during the end-season stage when the wheat crop is close to maturity. Overall, the results demonstrate the robustness of the proposed approach in estimating the spatial variation of ET using the Penman-Monteith method in conjunction with the on-field field stomatal conductance observations.

How to cite: Upreti, H. and Yadav, M.: Evaluation of Penman-Monteith estimates of evapotranspiration derived using field-collected stomatal conductance observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20031, https://doi.org/10.5194/egusphere-egu26-20031, 2026.

EGU26-21173 | Posters virtual | VPS23

Global Hot Spots of Climate Extremes from Composite Hazard Indices 

Natalia Zazulie, Francesca Raffaele, and Erika Coppola

Understanding the spatial distribution and intensity of climate-related hazards is essential for effective risk assessment and adaptation planning.  This study presents a comprehensive analysis of climate hazard indices applied across all IPCC reference regions, using all the available CMIP5-driven regional climate model (RCM) simulations at 25 km resolution over the CORDEX domains, together with Euro-CORDEX simulations at 12 km resolution. The objective is to identify climate hazard hot spots through the formulation of a composite hazard index. 

A subset of hazard indicators representing key climate extremes is selected. Temperature- and heat-stress–related hazards are characterized using TX90p (extreme maximum temperature), TN90p (extreme minimum temperature), and the NOAA Extended Heat Index (HI). Heavy precipitation and drought-related hazards are represented by RX1DAY (maximum 1-day precipitation), P99 (99th percentile of precipitation), and CDD (consecutive dry days).

The composite index integrates both the frequency and intensity of extremes and is computed at both regional and grid-point levels. A normalization approach is used to ensure comparability across regions with diverse climatic characteristics. Results reveal pronounced spatial heterogeneity in hazard intensity, highlighting regions where multiple hazards converge and amplify overall risk. This framework enables systematic identification of global and regional climate hot spots, offering insights into areas that may face heightened climate stress under current and projected conditions. By providing a consistent, region-wide assessment of hazard exposure, this study aims to support comparative climate risk analyses and inform policy-relevant decision-making for climate adaptation and resilience strategies at multiple scales.

How to cite: Zazulie, N., Raffaele, F., and Coppola, E.: Global Hot Spots of Climate Extremes from Composite Hazard Indices, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21173, https://doi.org/10.5194/egusphere-egu26-21173, 2026.

EGU26-21830 | ECS | Posters virtual | VPS23

Soil Moisture Based Calibration of a Hybrid Hydrological-Neural Network Model in Data Scarce Basins 

Khaoula Ait Naceur, El Mahdi El Khalki, Luca Brocca, Abdessamad Hadri, Oumar Jaffar, Mariame Rachdane, Vincent Simonneaux, Mohamed El Mehdi Saidi, and Abdelghani Chehbouni

Reliable river discharge simulation generally relies on observed streamflow data for model calibration; however, such observations are often uncertain or unavailable in data-scarce regions, limiting the applicability of conventional hydrological models. This study presents a hybrid modeling framework that uses soil moisture as an alternative calibration variable to improve discharge simulations in the absence of reliable streamflow observations. The framework couples a two-layer version of the daily lumped MISDc (Modello Idrologico Semi-Distribuito in continuo) hydrological model with a Feedforward Neural Network (FFNN), which is employed to enhance parameter calibration by exploiting soil moisture dynamics. The proposed approach is evaluated across three contrasting basins: Tahanaout in semi-arid Morocco, and Colorso (Italy) and Bibeschbach (Luxembourg) in temperate climates. Both in situ and ERA5-Land soil moisture datasets are used as calibration inputs. Model performance is assessed using multiple hydrological metrics, including Mean Absolute Error (MAE), Kling-Gupta Efficiency (KGE), and the correlation coefficient (R). Results show that the hybrid MISDc-FFNN framework substantially improves river discharge simulations compared to the traditional model. Across all basins, MAE is reduced by up to 61%, KGE increases by more than 200%, and R improves by up to 87%, with consistent performance gains observed for both observed and reanalysis-based soil moisture. These findings demonstrate the potential of soil moisture driven calibration strategies to enhance hydrological modeling in data-scarce environments, offering a viable pathway for improved water resources assessment and flood risk management where discharge observations are limited or unreliable.

 

Keywords: Soil moisture; river discharge simulation; hydrological modeling; machine learning; ERA5-Land; data-scarce regions; feedforward neural network

How to cite: Ait Naceur, K., El Khalki, E. M., Brocca, L., Hadri, A., Jaffar, O., Rachdane, M., Simonneaux, V., Saidi, M. E. M., and Chehbouni, A.: Soil Moisture Based Calibration of a Hybrid Hydrological-Neural Network Model in Data Scarce Basins, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21830, https://doi.org/10.5194/egusphere-egu26-21830, 2026.

Present-day practices of bridge piers design often employ group arrangements of piers in various configurations to modify flow dynamics and mitigate subsequent scour formation around the piers. These group arrangement configurations may vary in aspects of spacing ratio, number of piers, and orientations to alter the flow-structure interaction, and hence the scour development. Investigating the turbulent flow behaviour around various common group arrangements has been a topic of interest for researchers for a few years now. This study presents an experimental investigation aimed at comparing the equilibrium scour depth caused by various four-pier group arrangements. To assess the impact of spacing, the face-to-face distance between piers (G) was taken to values of D, 2D, and 3D, where D refers to the diameter of the circular pier. The scour patterns reveal that the maximum scour depth occurred when spacing G was equal to D. The equilibrium scour depth decreased with an increase in the pier spacing to 2D and 3D, corresponding to an approximate flow intensity of 0.9. The scour contours exhibit the impact of neighbouring piers and how it differs with an increase in pier spacing. Instantaneous velocity data were collected to derive the flow characteristics in the flow field. Velocity vectors depict the influence of different configurations on the flow pattern. The study provides an insight into the spacing effects on equilibrium scour, which can be useful in the design of pier group arrangements.

How to cite: Sahu, C.: Spacing Effect on the Equilibrium Scour and Flow Pattern around Four-Pier group in Different Configurations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22153, https://doi.org/10.5194/egusphere-egu26-22153, 2026.

EGU26-23043 | Posters virtual | VPS23

Analysis of Vector-Field Multifractal Cascades 

João Felippe Thurler Rondon da Fonseca, Daniel Schertzer, Igor da Silva Rocha Paz, and Ioulia Tchiguirinskaia
Multifractals provide a powerful framework to describe systems that exhibit variability over a wide range of scales together with strong intermittency. By encoding scale-dependent fluctuations through multiplicative cascades, multifractal models capture non-Gaussian statistics, heavy tails, and scale invariance in a compact and predictive manner. These properties have made multifractals particularly successful in the analysis of a wide variety of geophysical phenomena.
 
From the outset, multifractal fields have been formulated on domains of arbitrary dimension, allowing to represent space, space–time, or higher-dimensional parameter spaces. In contrast, the codomain of multifractal constructions has most often been restricted to scalar-valued fields. Although simpler for modeling and inference, the scalar setting omits directional information, anisotropy, and cross-component couplings that are essential in vector observations. Recent works, such as (Schertzer and Tchiguirinskaia 2020), have explored the use of Clifford algebras for constructing cascade generators, offering a natural algebraic framework to represent vector-valued multifractals while preserving their multiscale and symmetry properties.
 
In this work, we consider and simulate Clifford multifractal cascades as an extension of scalar models, capable of capturing directional variability and the internal geometry of multiscale fields. Rather than relying on a scalar stability exponent, we work in a framework where the stability can be encoded by algebra-valued or operator-like parameters, enabling anisotropic scaling and nontrivial coupling between different components of the Clifford field across scales.
 
To characterize the resulting operator-scaling structure, we extended the scalar analysis methods and developed inference methods that enable the direct estimation of multifractal parameters. Numerical experiments on synthetic cascades demonstrate that the proposed approach reliably recovers these parameters. The results demonstrate that extending multifractal analysis to vector-valued fields is both feasible and essential for the characterization of complex multiscale phenomena.

How to cite: Thurler Rondon da Fonseca, J. F., Schertzer, D., da Silva Rocha Paz, I., and Tchiguirinskaia, I.: Analysis of Vector-Field Multifractal Cascades, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23043, https://doi.org/10.5194/egusphere-egu26-23043, 2026.

GI1 – New Frontiers in Geoscience Instrumentation

EGU26-2752 | ECS | Posters on site | GI1.1

Comparative accuracy analysis of iPhone LiDAR applications for high-resolution 3D reconstruction 

Amjad Hamdan, Issa Loghmanieh, and László Bertalan

Accurate three-dimensional modeling of buildings and cultural heritage objects is crucial for applications such as modeling, engineering, and documentation. Traditional methods, such as Terrestrial Laser Scanning (TLS), provide high precision. The recent incorporation of LiDAR sensors into consumer smartphones, like iPhones, presents a cost-effective and accessible alternative. However, the accuracy and limitations of freely available mobile LiDAR applications have not been sufficiently quantified.

This research aims to quantitatively assess the geometric accuracy of iPhone LiDAR as a low-cost alternative for 3D modeling. Three free iPhone LiDAR applications, Modelar, 3D Scanner, and SiteScape, were evaluated across various study cases, focusing on small-scale heritage statues, indoor corridors, and exterior façades of a building. A geodetic reference network was established using a total station, leveler, and RTK GNSS to achieve high absolute accuracy for detailed comparison of the 3D point clouds. Tracking drift was minimized via standardized scanning procedures, maintaining a distance of less than five meters and moving slowly and methodically. The acquired point clouds were processed and compared using CloudCompare, incorporating noise filtering, control point alignment, Iterative Closest Point (ICP) refinement, and multiscale model-to-model (M3C2) analysis.

The results indicate RMS errors ranging from 1.34 cm for small heritage objects to 4.6 cm for building façades, with the Modelar application achieving the highest overall accuracy. Significant errors were concentrated around reflective surfaces such as glass windows, and the removal of these points improved geometric consistency by approximately 50%. All three applications produced point clouds suitable for small to medium-scale indoor and outdoor mapping; however, the 3D Scanner and SiteScape applications exhibited greater deviations, particularly in large or complex environments.

Freely available iPhone LiDAR applications, particularly Modelar, constitute a practicable low-cost option for expeditious centimeter-level 3D modeling in Building Information Modeling (BIM) and heritage documentation. Limitations persist for large-scale architectural elements and reflective materials, wherein TLS remains the benchmark for maximal precision. These results delineate the capabilities and constraints of iPhone LiDAR relative to geodetic references.

Issa Loghmanieh is funded by the Stipendium Hungarian scholarship under the joint executive program between Hungary and Iran.

How to cite: Hamdan, A., Loghmanieh, I., and Bertalan, L.: Comparative accuracy analysis of iPhone LiDAR applications for high-resolution 3D reconstruction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2752, https://doi.org/10.5194/egusphere-egu26-2752, 2026.

Field-based hyperspectral standoff measurements with a spectroradiometer encounter temporal limitations due to satellite overpass and optimum solar illumination requirements. Efficient sampling protocols, accurate targeting of the measured area, geolocation, repeatability, and rapid data acquisition are critical to the quality of field measurements. In this study we evaluate Spectral Evolution’s SensaProbe accessory used in conjunction with a high-resolution NaturaSpec Plus UV-Vis-NIR spectroradiometer. This accessory integrates an inclinometer, a laser for accurate targeting and distance calculation of the measured area, as well as a video camera for live visualization of the field-of-view of the target. Metadata such as GPS coordinates, solar angle, distance to target, inclination of the optic to the ground and picture of the field of view are automatically captured alongside hyperspectral data over the range of 350 to 2500nm. These capabilities are particularly valuable for satellite and airborne sensor validation, where precise spatial alignment and consistent acquisition geometry are essential for robust ground-truth comparisons. Our findings show that the consolidation of these measurements within one accessory reduced operator errors, enhanced metadata collection, streamlined acquisition workflows, and reduced the time required for accurate field measurements. These improvements suggest that integrated standoff systems like the SensaProbe can meaningfully enhance the quality and efficiency of hyperspectral datasets across many research fields such as environmental monitoring, precision agriculture, and remote sensing research.

How to cite: Woodman, M. and Venjean, N.: Innovative solution to improve the accuracy, repeatability, and efficiency of ground-based hyperspectral measurements with a spectroradiometer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2840, https://doi.org/10.5194/egusphere-egu26-2840, 2026.

EGU26-3050 | Orals | GI1.1

International collaboration for sustaining CTBTO International Monitoring System auxiliary seismic stations 

Chulalak Sundod, Irene Bianchi, Jose Pereira, Rizkita Parithusta, and Kadircan Aktas

Auxiliary seismic stations of the International Monitoring System (IMS) are an important part of the Comprehensive Nuclear-Test-Ban Treaty Organization’s (CTBTO) global monitoring network. While these stations contribute significantly to international monitoring capabilities, responsibility for their routine operation and sustainment rests with the host states. Many of these stations have limited national resources, making long-term sustainment challenging. They face issues such as ageing equipment, harsh environmental conditions, and evolving technical requirements. International collaboration is essential to ensure reliable operation. With financial support from Member States voluntary contributions (EU, Italy, Germany), CTBTO is able to work closely with national station operators to carry out site-specific upgrades and provide valuable training across multiple auxiliary stations.

The work achieved in auxiliary seismic stations in Bangladesh, Indonesia and Senegal demonstrates that international collaboration, combined with targeted instrumentation and infrastructure improvements, can significantly enhance the sustainability, reliability, and resilience of auxiliary seismic stations within the IMS network. Such collaborations also strengthen station operators’ sense of ownership and contribute meaningfully to capacity building. By supporting the CTBTO’s nuclear test detection and verification capabilities, these upgrades also reinforce global efforts in nuclear non-proliferation and disarmament under the Comprehensive Nuclear-Test-Ban Treaty (CTBT).

How to cite: Sundod, C., Bianchi, I., Pereira, J., Parithusta, R., and Aktas, K.: International collaboration for sustaining CTBTO International Monitoring System auxiliary seismic stations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3050, https://doi.org/10.5194/egusphere-egu26-3050, 2026.

We present a miniaturized, highly integrated MEMS optical accelerometer based on a diffraction-grating interferometric readout, targeting low-frequency, weak-motion measurements relevant to seismic observation. A novel mechanical architecture combined with a “sandwich” assembly approach enables a low fundamental resonance of 15.1 Hz while preserving a compact and robust package. At the system level, the laser source, MEMS interferometric module, and photodetector are integrated into a single enclosure measuring 4.5 cm × 3.5 cm × 3 cm, reducing alignment complexity and supporting field deployment.

Noise characterization demonstrates a self-noise of 2 ng/√Hz, indicating nanogram-level sensitivity in a small-form-factor instrument. We will describe the device concept, integration strategy, and dynamic/noise test methodology, and discuss how this accelerometer can complement existing seismic sensors for applications such as microtremor monitoring, dense temporary deployments, and near-field ground-motion characterization where size, power, and self-noise are critical constraints.

How to cite: sun, Z., zhou, W., cheng, Y., and yang, B.: A miniaturized, highly integrated MEMS diffraction-grating accelerometer with 15.1 Hz resonance and 2 ng/√Hz self-noise, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4815, https://doi.org/10.5194/egusphere-egu26-4815, 2026.

EGU26-6892 | Posters on site | GI1.1

Identification of the Sliding Surface of a Dormant Landslide Using UAV-Borne Low-Frequency Ground Penetrating Radar: The Melizzano Case Study (Southern Italy) 

Nicola Angelo Famiglietti, Bruno Massa, Paola Revellino, Giovanni Testa, Antonino Memmolo, Robert Migliazza, and Annamaria Vicari

Landslide analysis in vegetated and inaccessible areas represents a key challenge for hazard assessment and risk mitigation. This study presents the application of a UAV-borne low-frequency Ground Penetrating Radar (GPR) system to investigate the internal structure and deep geometry of an earth slide located in southern Italy. The GPR system is based on a Cobra Plug-in Sub-Echo 70 antenna operating in the 20–140 MHz frequency range and mounted on a multirotor UAV. The survey consisted of an east–west transect crossing the landslide body, flown at approximately 1 m above ground level due to dense vegetation about 60–70 cm high. To ensure precise navigation and stable flight altitude, the UAV was equipped with a high-precision GNSS system and a radar altimeter, enabling accurate terrain-following acquisition in complex topographic conditions.  The acquired radargram shows a coherent subsurface response down to an investigation depth of approximately 15 m. A laterally continuous, high-amplitude reflector is clearly visible at around 10 m depth and is interpreted as the main sliding surface controlling the gravity-driven process. Above this surface, zones of chaotic and heterogeneous reflections indicate disturbed stratigraphic units and reworked debris involved in deformation processes across the main body. The analysis highlighted a roto-translational kinematics in the upper part of the source area, as often observed in this type of landslide, evolving downslope into a predominantly translational movement. The central portion of the radargram exhibits more continuous sub-parallel reflectors, suggesting partial preservation of the original stratigraphic organization within the displaced material.  Despite the limited acquisition geometry, our results demonstrate that UAV-borne low-frequency GPR provides critical subsurface information for understanding gravity-driven processes. The identification of depth and geometry of landslide failure  surfaces  represents a key contribution to landslide susceptibility analysis, hazard evaluation for definition of effective risk mitigation and monitoring strategies.

How to cite: Famiglietti, N. A., Massa, B., Revellino, P., Testa, G., Memmolo, A., Migliazza, R., and Vicari, A.: Identification of the Sliding Surface of a Dormant Landslide Using UAV-Borne Low-Frequency Ground Penetrating Radar: The Melizzano Case Study (Southern Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6892, https://doi.org/10.5194/egusphere-egu26-6892, 2026.

EGU26-8191 | Posters on site | GI1.1

Design and experimental development of a portable instrument for measuring diffuse helium efflux in active volcanic systems  

Eleazar Padrón, Luis Bañares, Carlos Montero, Nemesio M. Pérez, Gladys V. Melián, Francisco Tabares, María Asensio-Ramos, Pedro A. Hernández, Pedro Recio, and Javier Cachón

Among the actions to be taken by any community threatened by volcanic activity to reduce the risk associated with volcanic hazards, a multidisciplinary approach to volcano monitoring is mandatory to optimize the early warning system for future volcanic eruptions. Such a multidisciplinary approach must be constantly updated with technological development. As part of this multidisciplinary approach to volcanic monitoring, attention to volcanic gases is one of the most important volcanic monitoring tool. The chemical composition of the gases emanating from a volcano, whether visible (through fumaroles and/or plumes) or non-visible (diffuse emissions), provides vital information on the degree of activity of a volcano. Monitoring and studying the behavior of volcanic gases as precursors of volcanic activity has attracted increasing interest from the scientific community. Portable instruments developed in the last 20 years allow measurement of larger gaseous species such as CO2, but in situ estimation of the emission of trace gases such as He is not possible to date, as the flux of this species is too low and would require too long accumulation times to distinguish changes in concentration inside the collection chamber. Among volcanic gases, helium (He) has unique characteristics as a geochemical tracer, as it is chemically inert and radioactively stable, non-biogenic, highly mobile and relatively insoluble in water. He flux is traditionally estimated following theoretical simulations, with strong limitations in the precision and accuracy of the He flux estimation. In this work we present a project that aims to overcome the technological limitations and develop a prototype to measure diffuse He emissions in situ in volcanic areas. “Portable” in this project is a key term, because the instrument must be suitable to be transported easily on the back of the volcanologist to complete surveys with tens of measurements each day. The project will take advantage of recent technological advances in two different technologies: (1) the miniaturization of quadrupole mass spectrometers (QMS), which have managed to drastically reduce their dimensions and weight; and (2) the possible spectrophotometric detection of He in trace levels. 

 

How to cite: Padrón, E., Bañares, L., Montero, C., Pérez, N. M., Melián, G. V., Tabares, F., Asensio-Ramos, M., Hernández, P. A., Recio, P., and Cachón, J.: Design and experimental development of a portable instrument for measuring diffuse helium efflux in active volcanic systems , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8191, https://doi.org/10.5194/egusphere-egu26-8191, 2026.

EGU26-9036 | Posters on site | GI1.1

Analytical solution of the influence of irregularly shaped loads in the near field on crustal deformation monitoring 

Wei Yan, Zirui Li, Anfu Niu, Lei Tang, Xian Lu, and Lina Zhai

Crustal movement and deformation monitoring are important methods for reflecting changes in crustal stress. Crustal deformation data can be used to accurately describe the movement and deformation characteristics of active blocks and their boundary zones, providing effective data constraints for earthquake prediction and scientific research. Crustal deformation monitoring mainly includes crustal movement monitoring (such as Global Navigation Satellite System (GNSS) observations), surface strain monitoring (such as borehole strain observations), and surface tilt monitoring (such as vertical pendulum tilt observations). The high-precision and high temporal resolution data generated are widely used in the study of slow earthquakes, volcanic activity, and earthquake precursors. Given the close relationship between geophysical instruments and observation environments, crustal deformation monitoring instruments can not only record structural signals, but also interference signals caused by changes in surrounding loads. This article is based on the analysis displacement solution caused by the point load model, and derives formulas for calculating the surrounding tilt field and strain field, providing a theoretical basis for the quantitative calculation of the influence of surrounding loads in crustal deformation monitoring. In addition, this article also proposes a method for calculating the strain effects of two-dimensional and three-dimensional irregular shaped loads. Finally, based on the four component borehole strain observation data from Guza borehole strainmeter and the observation data of the surrounding river water level, the applicability of this analytical solution in quantitatively calculating the degree of influence of irregular load models in the surrounding area was verified under the conditions of setting the surrounding medium parameters (elastic modulus and Poisson's ratio). The results indicate that: (a) for the two-dimensional irregular shaped load model problem, vector superposition calculation can be performed after load scattering; (b) For the problem of three-dimensional irregular shaped load models, different weights can be assigned to scattering points after load scattering, and the two-dimensional irregular shaped load method can be used for calculation. The convergence process during vector superposition proves the correctness and feasibility of this method. This study provides a research foundation for the quantitative analysis of the influence of surrounding load interference in crustal deformation monitoring; (c) There is a high possibility that the data disturbance information of the four component drilling strain observation data at Guzan Station in summer is affected by the disturbance of the water level data of nearby rivers. This research work can quantitatively explain the degree of influence of load type interference factors on high-precision geophysical observation data, providing a quantitative interpretation scheme for the extraction of earthquake precursor anomalies.

Fund support: Ningxia Natrual Science Foundation Project (2024AAC03436); National Natural Science Foundation of China (41704062); National Key Research and Development Program of China (2021YFC3000705-06).

Figure 1 Example of the influence of irregularly shaped loads in the near field. In the figure: (a) represents the positional relationship between the Guzan borehole strainmeter and the Dadu River; (b) Representing the comparison of the changes in actual observed data with the results of irregular load model calculations.

How to cite: Yan, W., Li, Z., Niu, A., Tang, L., Lu, X., and Zhai, L.: Analytical solution of the influence of irregularly shaped loads in the near field on crustal deformation monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9036, https://doi.org/10.5194/egusphere-egu26-9036, 2026.

EGU26-9092 | Posters on site | GI1.1

Drone magnetic surveys of Aeolian Islands (Italy) hydrothermal areas within IRGIE project 

Rosalba Napoli, Emanuela De Beni, Massimo Cantarero, Antonino Sicali, Gilda Currenti, Barbara Cantucci, and Monia Procesi

Unmanned aircraft vehicle (UAV) and airborne magnetometers have recently emerged as new technology to gather, in a productive and economical way, high-resolution magnetic data. In volcanic environments, taking advantage of the strong magnetization contrasts of adjacent rock formations, magnetic field measurements can detect and characterize the main subsurface structural features and indicate areas of hydrothermal alteration, or highlight thermal anomalies. Magnetometer-equipped drones have advantages in high maneuverability and hover ability and are able to carry out large-scale magnetic surveys in areas that are difficult to access due to complex ground conditions and large topographical fluctuations or that would pose a potential hazard to operators.

Between 2024 and 2025, aeromagnetic surveys were conducted by UAV within the IRGIE project for the first time at Aeolian Islands (Italy) to identify possible areas of different magnetization potential related to hydrothermal fluid circulation. In particular, the most significant geochemistry sites have been investigated at Lipari, Salina, Panarea and Vulcano Islands. The airborne magnetic surveys were conducted using the Matrice 300 UAV with a MagArrow sensor, a laser pumped cesium total field scalar magnetometer, collecting magnetic data at a 1000 Hz sample rate synchronized on-board GPS (1 Hz sample rate). The high spatial resolution offered by the use of low-altitude drones proved essential for mapping the magnetic anomaly in detail and deducing the distribution of magnetization intensity in the investigated regions. The upcoming interpretation of acquired magnetic data, to be integrated with geophysical and geochemical data will may contribute to the development of conceptual models of geothermal circulation in the investigated areas.

How to cite: Napoli, R., De Beni, E., Cantarero, M., Sicali, A., Currenti, G., Cantucci, B., and Procesi, M.: Drone magnetic surveys of Aeolian Islands (Italy) hydrothermal areas within IRGIE project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9092, https://doi.org/10.5194/egusphere-egu26-9092, 2026.

Maritime anomaly detection with Orthogonal Time-Frequency Space (OTFS) sensing commonly involves assessing individual delay-Doppler (DD) maps using set thresholds, Constant False Alarm Rate (CFAR) methods, or detectors that learn frame by frame. However, sea clutter is naturally unstable, changing with sea conditions, wind, and movement of the platform. It frequently generates brief bursts that may seem like anomalies in a single DD image, particularly when Doppler is spreading. Consequently, false positives can change, and detection accuracy becomes unreliable as conditions change. A significant drawback of many OTFS sensing systems is that they handle each DD map in isolation, failing to utilize the temporal consistency of actual anomaly signatures. This makes it hard to differentiate between lasting anomalies and temporary clutter changes in tough situations.

We introduce a spatio-temporal OTFS sensing system that detects objects using a brief series of delay-Doppler maps, instead of just one frame. The receiver creates a DD "cube" by arranging L successive OTFS frames (usually L = 3-100) and uses motion-sensitive Doppler alignment. This involves estimating the general clutter Doppler shift for each frame (for instance, by tracking the Doppler centroid or ridge) and compensating for this shift before combining the frames temporally. The aligned DD cube is then analyzed by a spatio-temporal detector, such as a streamlined 3D U-Net (a 3D convolutional encoder-decoder) or a 2D U-Net enhanced with a Convolutional Long Short-Term Memory (ConvLSTM) bottleneck or temporal attention. Training employs standard DD representations with Binary Cross-Entropy (BCE) plus Dice supervision, along with a temporal-consistency regularizer to reduce flickering detections. Potential peaks are identified using Non-Maximum Suppression (NMS) and confirmed using a track-before-detect persistence gate (for example, requiring detections in 2 of the last 3 frames along a physically reasonable drift), boosting dependability without needing manual adjustments. The suggested method, which considers both space and time, should offer small but reliable enhancements in challenging environments compared to single-image detection. These environments include situations with a poor signal-to-noise ratio, significant Doppler spread, and changes in sea conditions. In these cases, we aim for an increase in the F1-score of +0.01 to +0.03 (in situations where performance is not already at its peak) and a relative decrease of 15–25% in false positives while maintaining the same recall rate. This is mainly achieved through motion-compensated temporal fusion and persistence validation. Additionally, across different sea conditions, we seek a 10–20% relative decrease in performance variation, which would indicate greater resilience and more consistent operational performance.

The suggested system enhances OTFS maritime sensing in the face of Doppler-dispersive, nonstationary sea clutter by integrating motion-compensated temporal alignment with DD-cube detection and persistence-based confirmation. This leads to more consistent anomaly detection, avoiding the need for threshold adjustments for each specific situation.

Acknowledgment: This research was supported by the Korea Institute of Marine Science & Technology Promotion (KIMST) funded by the Ministry of Oceans and Fisheries, Korea (RS 2021-KS211502, RS-2022-KS221620).

How to cite: Yoo, J. and Hussain, K.: Motion-Compensated Spatio-Temporal Delay–Doppler Cube Detection for Robust Maritime OTFS Sensing under Nonstationary Sea Clutter, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9510, https://doi.org/10.5194/egusphere-egu26-9510, 2026.

EGU26-9720 | Orals | GI1.1

Presence of environmental mercury in a former Tartessian sanctuary: La Bienvenida (Almodóvar del Campo, Spain). 

Pablo Higueras, Mar Zarzalejos, Luis Mansilla, Germán Esteban, Oscar Avalos, and Patricia Hevia

This study is based on samples recovered from an archaeological context dating back to the 6th century BC, belonging to a Tartessian sanctuary identified at the La Bienvenida site (Almodóvar del Campo, Ciudad Real, Spain). The aim of the research is to determine whether there was anthropic use of Almadén cinnabar at this time at a site that, centuries later, would become the location of the city of Sisapo. This city was mentioned by Pliny the Elder (Nat. Hist. 33, 118) as the main supplier of cinnabar to Rome.

The analyses were performed using Zeeman effect atomic absorption spectrometry, following pyrolysis of the samples. We analysed the archaeological pieces, as well as the patina of detrital materials on their surfaces. The results show that Hg is present in these detrital materials, reaching concentrations of up to 350 mg kg-1. This material is undoubtedly a clear indication of the widespread distribution of the element in the environment of the area, as it corresponds to the adhesion of local soil to the pieces due to the collapse of the building and its burial. In conclusion, we can deduce that, during the corresponding historical period, Hg extracted from the Almadén mine was processed in this locality.

How to cite: Higueras, P., Zarzalejos, M., Mansilla, L., Esteban, G., Avalos, O., and Hevia, P.: Presence of environmental mercury in a former Tartessian sanctuary: La Bienvenida (Almodóvar del Campo, Spain)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9720, https://doi.org/10.5194/egusphere-egu26-9720, 2026.

EGU26-10503 | Posters on site | GI1.1

A comparison of 3D MWT Reconstruction Models for UAV-based GPR 

Ilaria Catapano, Giuseppe Esposito, Giovanni Ludeno, Carlo Noviello, Francesco Soldovieri, and Gianluca Gennarelli

Ground Penetrating Radar (GPR) [1-2] is a well-established geophysical technique for high-resolution subsurface investigations and is increasingly integrated with UAV platforms to enable rapid, flexible, and non-invasive surveys [3]. This contribution presents a comparative analysis of two three-dimensional microwave tomography (MWT) approaches for processing UAV-GPR multimonostatic data. The approaches differ for the adopted scattering model: the Interface Reflection Point 3D (IRP3D) model [4-5] and the Equivalent Permittivity 3D (EP3D) model, previously proposed for 2D imaging in [6]. The approaches are compared in terms of spatial resolution by inverting full-wave simulated data referred to a point like scatterer and the effect of data spacing as well as the irregular distribution is examined. Experimental data collected in laboratory-controlled conditions are considered to validate the expected performance. Furthermore, results referred to on field data acquired at the Altopiano di Verteglia (Avellino, Italy), are provided. The reconstruction capabilities are quantitatively assessed through image-based metrics, including image contrast and entropy, highlighting strengths and limitations of each approach. The results provide insights into the suitability of advanced 3D MWT algorithms for UAV-supported GPR surveys and contribute to the development of robust processing workflows for drone-based subsurface imaging.

[1] D. J. Daniels, Ground Penetrating Radar. Hoboken, NJ: Wiley, 2005.

[2] R. Persico, Introduction to Ground Penetrating Radar: Inverse Scattering and Data Processing. Hoboken, NJ: Wiley, 2014.

[3] C. Noviello, G. Gennarelli, G. Esposito, G. Ludeno, G. Fasano, L. Capozzoli, F. Soldovieri, I. Catapano, “An Overview on Down-Looking UAV-Based GPR Systems,” in Remote Sensing, 2022, 14(14):3245. https://doi.org/10.3390/rs14143245.

[4] G. Gennarelli, C. Noviello, G. Ludeno, G. Esposito, F. Soldovieri and I. Catapano, "Three-Dimensional Ray-Based Tomographic Approach for Contactless GPR Imaging," in IEEE Transactions on Geoscience and Remote Sensing, vol. 61, pp. 1-14, 2023, Art no. 2000614, doi: 10.1109/TGRS.2023.3250740.

[5] G. Esposito, G. Gennarelli, F. Soldovieri and I. Catapano, "Effective 3-D Contactless GPR Imaging: Experimental Validation," in IEEE Geoscience and Remote Sensing Letters, vol. 21, pp. 1-5, 2024, Art no. 3509005, doi: 10.1109/LGRS.2024.3451729.

[6] G. Ludeno, L. Capozzoli, E. Rizzo, F. Soldovieri, I. Catapano, “A Microwave Tomography Strategy for Underwater Imaging via Ground Penetrating Radar,” in Remote Sensing, 2018, 10, 1410. https://doi.org/10.3390/rs10091410.

How to cite: Catapano, I., Esposito, G., Ludeno, G., Noviello, C., Soldovieri, F., and Gennarelli, G.: A comparison of 3D MWT Reconstruction Models for UAV-based GPR, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10503, https://doi.org/10.5194/egusphere-egu26-10503, 2026.

EGU26-11805 | Posters on site | GI1.1

LZER0-MOB: cost-effective GNSS for temporary monitoring 

David Zuliani, Alessio Compagno, Paolo Fabris, Francesco De Giorgi, Simone Galvi, Andrea Magrin, Enrico Magrin, Alberto Pastorutti, Lavinia Tunini, Piero Ziani, and Sonia Zorba

OGS has been developing and producing cost-effective GNSS technology devices and systems in collaboration with the private sector since 2015. These systems, called LZER0, have been efficiently applied to landslide monitoring, also in collaboration with local administrations and the Regional Civil Protection. In recent years, the development of LZER0 has received new impetus from the PNRR Geoscience IR project.

We have developed a new adaptation of the LZER0 device for temporary monitoring, called LZER0-MOB. It addresses the specific needs of temporary monitoring, which may be carried out in emergency conditions, such as user-friendliness and reduced consumption and weight.

We have implemented a mobile infrastructure ready to be activated in case of emergencies due to geological hazards, consisting of a pool of LZER0-MOB stations. This infrastructure, which benefits from the low cost of these devices, will expand monitoring capabilities during emergencies to support civil protection activities and will be integrated into existing infrastructures. It will also enable continuous monitoring of areas of specific interest after the emergency phases.

In the first prototypes, the usability of LZER0 was limited by configuration management and data distribution, which were based on command line interaction. In addition, each station had to be managed individually. For this reason, we have improved the user interface for managing the cost-effective devices (as single stations or as station networks) and for querying and viewing data in real time. We have also developed an automatic system to manage the initial installation of software and its remote updating. These software improvements will enhance the usability of these systems for end users.

The technical diagrams of the instruments and the developed software are released under the CC BY 4.0 license through the repository of LZER0 on github (https://github.com/OGS-GNSS/LZER0) and the Geosciences IR research infrastructure portal (https://geosciences-ir.it/infrastruttura/).

Acknowledgements

Funded by European Union - NextGenerationEU - Mission 4 “Education and Research” - Component 2 “From Research to Business” - Investment 3.1 “Fund for the realization of an integrated system of research and innovation infrastructures” - Project IR0000037 - GeoSciences IR - CUP I53C22000800006. We thank Lunitek SRL for the collaboration provided in the creation of the instrumentation.

How to cite: Zuliani, D., Compagno, A., Fabris, P., De Giorgi, F., Galvi, S., Magrin, A., Magrin, E., Pastorutti, A., Tunini, L., Ziani, P., and Zorba, S.: LZER0-MOB: cost-effective GNSS for temporary monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11805, https://doi.org/10.5194/egusphere-egu26-11805, 2026.

EGU26-12457 | Posters on site | GI1.1

Drone Based Field Measurements of a Lightweight Electromagnetic Induction System (SELMA-TF) for Agricultural Applications 

Markus Dick, Achim Mester, Egon Zimmermann, Peter Wüestner, Michael Ramm, Benedikt Scherer, Julie Bernard, Salar Saeed Dogar, Carsten Montzka, Cosimo Brogi, Johan Alexander Huisman, and Ghaleb Natour

Precision agriculture is increasingly using rapid and non-invasive methods to characterise soil properties and monitor field status, with the aim of enabling efficient and sustainable management. Electromagnetic induction (EMI) can be used to rapidly measure the electrical conductivity of the soil and thereby provide information about the soil complexity, water content dynamics, and nutrient availability. The use of Unmanned Aerial Vehicles (UAVs) allows measurements of soil properties on cultivated land and makes the method independent from field conditions.
We developed a lightweight, scalable EMI sensing platform with a fast data acquisition for deployment on hexacopters in the 25 kg class. The system has one transmitter and four receivers with variable coil pair distances of 1.5 m, 1.9 m, 2.3 m, and 2.7 m. The EMI system weighs less than 5 kg and allows a measurement time of approximately 15 minutes with a fully charged 100 Wh battery from a DJI600 UAV. The apparent conductivity values are recorded at a measurement rate of 10 Hz. WLAN communication, MQTT-based protocols, a TimeScale database and a web-based measurement interface enable real-time display of the data.
During the initial test and evaluation phase, EMI measurements are carried out using a UAV at several defined measurement points and at multiple elevation levels across the test field near Jülich, Germany. The goal of the test was to (a) identify the UAVs electromagnetic interference on EMI measurements at different distances from the drone, to (b) assess the feasibility of vertical measurements at different altitudes, to (c) determine reference conductivity values using a commercial EMI system at several positions on the ground, to (d) record corresponding housekeeping data from DGPS and onboard position sensors and to (e) perform a potential offset calibration based on the acquired datasets.

How to cite: Dick, M., Mester, A., Zimmermann, E., Wüestner, P., Ramm, M., Scherer, B., Bernard, J., Dogar, S. S., Montzka, C., Brogi, C., Huisman, J. A., and Natour, G.: Drone Based Field Measurements of a Lightweight Electromagnetic Induction System (SELMA-TF) for Agricultural Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12457, https://doi.org/10.5194/egusphere-egu26-12457, 2026.

EGU26-12703 | ECS | Posters on site | GI1.1

A Route Optimization Framework for Vehicle-Based Mobile Remote Sensing  

Can Topaclioglu, Louis Trinkle, John Anders, Solveig Landmark, Martin Schrön, Peter Dietrich, and Hendrik Paasche

Optimizing the informational return of measurements along existing road networks is a big challenge for real life data acquisition. Here, informational return describes the effectiveness of a survey in capturing the spatial variability of the target variable, ensuring that measurements provide maximal knowledge and minimize uncertainty when used to generate spatial maps or inform predictive models. In this study we develop a two-stage survey design framework that fuses auxiliary spatial data with road network data and formulates route planning as a combinatorial optimization problem. By integrating a fuzzy-clustered representation of the survey area heterogeneity with the road network, we identify map grid nodes reachable by a vehicle. Information values are assigned to individual road segments using fuzzy membership values and Shannon Entropy. Informative segments are selected, and the most informative pathways between them are constructed using Dijkstra’s Algorithm. An Information-rich initial route is then generated using Ant Colony Optimization (ACO).

To further economize this initial route, spatial coverage is characterized by computing a convex hull in the auxiliary data space. A subset of map grid nodes is heuristically selected to preserve most of the convex hull volume while keeping the computational cost manageable. The shortest paths between road segments covering these nodes are determined with the A* algorithm.  The ACO is applied to construct the final economized route that is both information-rich and distance-optimized.

The framework is evaluated using a large-scale case study based on mobile Cosmic Ray Neutron Sensing (CRNS) soil moisture measurements over a 4500 km2 area in northeastern Germany. Compared to an empirically designed route of similar length, the optimized route substantially reduces uncertainty in regression-based soil moisture regionalization (i.e., map generation) while significantly improving spatial coverage of the survey area, data collection efficiency, and data quality. The proposed approach provides a systematic alternative to convenience-based sampling strategies commonly used in Earth and environmental sciences.

How to cite: Topaclioglu, C., Trinkle, L., Anders, J., Landmark, S., Schrön, M., Dietrich, P., and Paasche, H.: A Route Optimization Framework for Vehicle-Based Mobile Remote Sensing , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12703, https://doi.org/10.5194/egusphere-egu26-12703, 2026.

EGU26-12843 | Orals | GI1.1

Uas-Based Multitemporal Remote Sensing Of The 2021 Tajogaite Eruption (La Palma Island, Spain) 

Riccardo Civico, Tullio Ricci, Ulrich Kueppers, Wolfgang Stoiber, Víctor Ortega-Ramos, Iván Cabrera-Pérez, Monika Przeor, Jacopo Taddeucci, Piergiorgio Scarlato, and Luca D'Auria

Volcanic eruptions shape the landscape. While some events may locally cause mass loss following e.g. gravitational failure, explosive excavation or collapse following magma withdrawal, constructive processes are by far the most abundant: volcanic deposits can create new land, cover the landscape and create new cones around the vents.

The 2021 Tajogaite eruption (La Palma, Spain, 19 September - 13 December 2021) produced a cinder cone that was initially (January 2022) 187 m taller than the pre-eruption topography. The cone is likely welded in some parts but is covered by unconsolidated deposits. This volcanic edifice offered a unique opportunity to monitor its shape evolution after the eruption.

To this end, we are using six datasets of UAS surveys with optical cameras between March 2022 and July 2024. Structure-from-Motion (SfM) photogrammetry allowed us to produce high-resolution (up to 0.2 m/pixel) DSMs (Digital Surface Models) and orthophotomosaics (up to 0.1 m/pixel). This unprecedented and unique dataset, moreover, allows us to constrain these changes at high temporal and spatial resolution. Over the course of our observation period, our conservative approach reveals that the cone "shrank" by more than 10 m in height and lost almost 1*106 m3 of volume. The rate of these changes was highest at the beginning (6,2 cm height loss per day between 28 January and 21 March 2022) and declined exponentially. Towards the end of the observation period reported here (7 August 2023 to 18 July 2024), the average rate was 0,3 cm per day. These quantifications showed that surface processes (wind, rain) accounted for approximately 10% of volume loss, with approximately 75*103 m3 being redeposited at the base of the cone. Satellite data show that there is no significant westward movement of the entire cone. Accordingly, most of the observed shape change of the Tajogaite cone is due to intrinsic processes, such as 1) decrease of magmatic pressure, 2) volume loss due to outgassing and cooling and 3) compaction of tephra deposits. The contribution of these individual processes will be discussed.

How to cite: Civico, R., Ricci, T., Kueppers, U., Stoiber, W., Ortega-Ramos, V., Cabrera-Pérez, I., Przeor, M., Taddeucci, J., Scarlato, P., and D'Auria, L.: Uas-Based Multitemporal Remote Sensing Of The 2021 Tajogaite Eruption (La Palma Island, Spain), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12843, https://doi.org/10.5194/egusphere-egu26-12843, 2026.

Low-cost seismic instruments, such as Raspberry Shake sensors, are increasingly deployed to complement traditional seismic networks and enable applications ranging from network densification and education to low-cost forensic seismology monitoring and local early warning; however, systematic performance comparisons with broadband stations remain essential.

The Cadí station, part of the CA Catalan network and operated by LEGEF-IEC, is located in the eastern Pyrenees, a region of moderate seismicity that is of particular relevance for seismic hazard assessment and emergency planning in Catalonia. CADI is installed inside an abandoned tunnel that provides stable thermal conditions and protection from atmospheric effects; despite this isolation, the site exhibits medium-to-low ambient noise levels due to the presence of nearby transportation infrastructure. In general this emplacement provides favorable conditions for instrument comparison.

In this study, we assess the data quality and detection capabilities of a Raspberry Shake RS3D short-period sensor through a direct comparison with broadband instrumentation (Guralp CMG3T and Centaur digitizer) at the CADI site. Before the comparison period, only the low-cost sensor was active due to broadband maintenance; afterward, both instruments ran together, allowing direct comparison and validation of the prior CADI recordings

Continuous seismic data recorded between September 2024 and April 2025 were analyzed and compared using cumulative Power Spectral Density (PSD) spectra and Root Mean Square (RMS) amplitude estimates, using part of the SeismoRMS free software (Lecocq et al., 2020). Broadband data were compared with Raspberry Shake recordings during their overlapping operational period to assess noise levels, frequency response, and sensitivity across relevant seismic bands. PSDs were evaluated relative to the New Low and High Noise Models to characterize baseline performance.

Results show that both instruments exhibit comparable spectral behavior above 0.1 Hz, capturing similar noise patterns and anthropogenic signals in the high-frequency band (10–40 Hz). However, the broadband sensor demonstrates superior performance at lower frequencies, reliably recording signals below the narrowband instrument’s response range.

This difference becomes critical for the detection of teleseismic events, which are only clearly recorded by the broadband station, while both sensors adequately capture local and regional earthquakes. These findings highlight the strengths and limitations of low-cost seismic instrumentation and confirm that Raspberry Shake sensors can effectively complement broadband networks for local and regional monitoring, while broadband stations remain essential for comprehensive seismic observations.

 

Reference

Lecocq, T., Massin, F., Satriano, C., Vanstone, M., & Megies, T. (2020). SeismoRMS - A simple python/jupyter notebook package for studying seismic noise changes (1.0). Zenodo. https://doi.org/10.5281/zenodo.3820046

 

How to cite: Ladero, J., Tapia, M., and Suriñach, E.: Performance of a Broadband Seismic Station Versus a Co-located Raspberry Shake: Implications for Low-Cost Seismic Monitoring , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13189, https://doi.org/10.5194/egusphere-egu26-13189, 2026.

EGU26-17894 | Posters on site | GI1.1

The Güralp Stratis: A Commercial Six-Degree-of-Freedom Seismometer for Ground Motion and Structural Monitoring  

Federica Restelli, James Lindsey, Antoaneta Kerkenyakova, Jamie Calver, Krystian Kitka, Neil Watkiss, and Phil Hill

Traditional research-grade three-component seismic sensors are inherently sensitive to both translational ground motion and rotational (tilt) motion, particularly on the horizontal components. The outputs of traditional seismometers represent a sum of rotation and displacement information. As a result, recorded signals represent a superposition of displacement and rotation, even though most processing and interpretation workflows assume purely translational motion. This limitation becomes increasingly important for applications involving near-field ground motion, ground-structure interaction, and structural response monitoring, where rotational effects can significantly influence observed building and infrastructure dynamics. Recent advances in sensor technology are now allowing accurate and precise discrimination between translational and rotational motion.  

Stratis is the world’s first integrated seismic sensor to provide simultaneous, co-located measurements of all six degrees of freedom, delivering concurrent velocity (m/s) and rotational velocity (rad/s) outputs in the Z, N, and E directions. By measuring all six degrees of freedom at a single point, Stratis avoids the spatial differencing and approximation errors associated with multi-instrument rotational estimates. The availability of co-located rotational measurements enables correction for tilt-induced contamination in translational records, supporting the derivation of rotation-corrected displacement signals and improving the fidelity of ground motion and structural response observations. By integrating rotational and translational sensing into a single compact instrument, the installation process is also greatly simplified, thereby enabling wider access to rotational seismic data. This supports interdisciplinary applications spanning seismology, structural engineering, and seismic risk mitigation, including post-event damage assessment, long-term monitoring of structural health, and improved characterization of earthquake ground motion relevant to robust infrastructure design. 

How to cite: Restelli, F., Lindsey, J., Kerkenyakova, A., Calver, J., Kitka, K., Watkiss, N., and Hill, P.: The Güralp Stratis: A Commercial Six-Degree-of-Freedom Seismometer for Ground Motion and Structural Monitoring , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17894, https://doi.org/10.5194/egusphere-egu26-17894, 2026.

EGU26-18427 | ECS | Posters on site | GI1.1

Ultra-high performance gyroscopes for future X-ray interferometer missions 

Andreas Brotzer, Felix Bernauer, Frédéric Guattari, Leszek R. Jaroszewicz, Anna T. Kurzych, Carlos L. Garrido Alzar, Arnaud Landragin, Damien Piot, and Sebastien De Raucourt

X-ray interferometry holds the potential to image astronomical objects with unprecedented, microarcsecond (μas) resolution, where 1 μas corresponds to 4.8 prad. This target resolution imposes extreme requirements for the accuracy of the spacecraft‘s attitude measurement when operating the X-ray interferometer.

Typically, the orientation of the spacecraft is measured using three single-axis gyroscopes that measure the Euler angles (yaw, pitch and roll) in a spacecraft-fixed coordinate frame. These measurements can be complemented by a star tracker as an absolute reference. Gyroscopes that are capable of determining the orientation with the required accuracy and stability needs to outperform the current high-performance navigation-grade gyroscopes by several orders of magnitude.

High-accuracy rotation angle and rotation rate measurements become increasingly important in many scientific fields: (1) Seismologists want to observe the local rotation from elastic and non-elastic deformation caused by earthquakes to fully observe the seismic wavefield. (2) The next generation of gravitational wave detectors relies on high-precision rotation measurements for enhanced active seismic noise isolation and Newtonian noise mitigation. (3) Geodesists want to measure the Earth’s rotation rate and its variations with Earth-bound instruments. All these applications require gyroscopes with a sensitivity in the range of 1 prad/s/√Hz to 1 nrad/s/√Hz, covering a frequency range from below 0.01 Hz to up to 100 Hz.

This contribution presents (1) a compilation of requirements for a sensor suite to comply with the mission needs, (2) an assessment of the state-of-the-art gyroscope technologies (e.g. fiber-optic gyroscopes, ring-laser gyroscopes, cold atom gyroscopes and mechanical gyroscopes), comprising their scaling parameters as well as technological gaps, and (3) a road map to an ultra-high performance sensor suite for 2030+.

How to cite: Brotzer, A., Bernauer, F., Guattari, F., Jaroszewicz, L. R., Kurzych, A. T., Garrido Alzar, C. L., Landragin, A., Piot, D., and De Raucourt, S.: Ultra-high performance gyroscopes for future X-ray interferometer missions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18427, https://doi.org/10.5194/egusphere-egu26-18427, 2026.

EGU26-19517 | Orals | GI1.1

Drone-based Magnetic Surveys for Lava Tube Detection in Volcanic Terrains: Preliminary Results from Etna and Vesuvius 

Pietro Tizzani, Filippo Accomando, Andrea Barone, Andrea Vitale, Susi Pepe, Giuseppe Solaro, and Raffaele Castaldo

Magnetic surveying is a key geophysical technique for detecting subsurface structures due to its sensitivity to lithological and structural variations. Recent advances in lightweight, high-sensitivity magnetometers have enabled their integration with UAV platforms, allowing rapid, high-resolution data acquisition in complex terrains. This approach improves logistical flexibility, reduces survey times, and ensures safe, non-invasive investigations in areas otherwise difficult to access.

Within the PRORIS initiative (https://www.proris.it/), our team conducted UAV-based magnetic surveys to identify and characterize lava tubes in volcanic environments, focusing on Mount Etna and Mount Vesuvius. These campaigns aimed primarily at testing and validating innovative geophysical methodologies through collaboration among research institutions.

The surveys employed different magnetometric systems, including MagArrow and Magnimbus (in gradiometric configuration), mounted on UAVs. Multiple acquisition strategies were explored, such as varying flight altitudes and sensor-to-platform distances, to assess their impact on signal quality and anomaly resolution. UAV deployment proved essential for achieving dense coverage and safe operations in steep, inaccessible areas.

Preliminary results revealed distinct magnetic anomalies consistent with subsurface lava tubes, some confirmed by historical speleological data. However, interpretation was complicated by partially collapsed tubes and sediment infill, which often share magnetic properties with surrounding rock, reducing anomaly contrast. These challenges highlight the importance of optimizing sensor configurations and survey design.

The primary goal of these initial campaigns was methodological: evaluating the effectiveness of different magnetometric setups and acquisition approaches for lava tube detection. Future work will focus on 3D modeling of detected structures using magnetic inversion techniques and integrating magnetometry with complementary geophysical methods, particularly ground-penetrating radar (GPR). This multi-sensor approach is expected to enhance resolution and reliability of subsurface models, supporting applications in volcanic studies and analog environments.

By combining UAV-borne magnetometry with advanced processing strategies and other geophysical tools, this research contributes to the development of robust remote sensing techniques for subsurface exploration. These efforts expand the capabilities of geophysical investigations in challenging terrestrial settings and provide a foundation for future applications in planetary analog studies.

How to cite: Tizzani, P., Accomando, F., Barone, A., Vitale, A., Pepe, S., Solaro, G., and Castaldo, R.: Drone-based Magnetic Surveys for Lava Tube Detection in Volcanic Terrains: Preliminary Results from Etna and Vesuvius, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19517, https://doi.org/10.5194/egusphere-egu26-19517, 2026.

EGU26-19724 | ECS | Posters on site | GI1.1

Multiscale analysis of geophysical data in the framework of PRORIS and MARS-LAVA projects. 

Andrea Barone, Andrea Vitale, Filippo Accomando, Francesco Mercogliano, Raffaele Castaldo, Giuseppe Solaro, Susi Pepe, Ilaria Catapano, Ugo Cortesi, Roberto Orosei, and Pietro Tizzani

In the framework of the planetary missions, the human exploration of the Martian surface is becoming a priority. The pathway to Mars is rooted through the development of various space missions of increasing complexity, which will lead to a long-term and sustainable human presence on the Moon. The Moon is therefore an intermediate and fundamental step for testing most of the new technologies required for sustainable human exploration of deep space.

We here present an overview of two Italian National projects dedicated to the development of geophysical technologies for planetary exploration, including the “PROgramma di RIcerca Spaziale di base (PRORIS)” project, funded by the Italian Ministry of University and Research (MUR) and whose management has been assigned to the National Research Council of Italy (CNR) and the National Institute for Astrophysics (INAF), and the “Martian Analysis of Resources and Structures: Lava tubes, neAr-surface ice and aquifers Visibility and Assessment (MARS-LAVA)” project, led by CNR and INAF.

The PRORIS project is mainly related to the Moon exploration with different activities for the development of methodologies and research prototypes, and the validation of the developed technologies in terrestrial analog environments. The MARS-LAVA project instead aims at developing, optimizing and testing a suite of geophysical sensors with high potential for Mars exploration, and to develop analysis techniques based on data fusion/integration and modeling, Both the projects involve the use of magnetometric and electromagnetic geophysical methods.

In this contribution,  we dedicate a particular focus to the multiscale analysis of magnetometric data for studying lava tubes, presenting the preliminary results of magnetometric surveys carried out at Italian lava tubes test-sites.

These results underline the potential of the multiscale analysis of magnetometric data in the framework of the planetary exploration and the challenges that need to be overcome.

How to cite: Barone, A., Vitale, A., Accomando, F., Mercogliano, F., Castaldo, R., Solaro, G., Pepe, S., Catapano, I., Cortesi, U., Orosei, R., and Tizzani, P.: Multiscale analysis of geophysical data in the framework of PRORIS and MARS-LAVA projects., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19724, https://doi.org/10.5194/egusphere-egu26-19724, 2026.

EGU26-19830 | ECS | Orals | GI1.1

Arithmetic Integration of GPR and Magnetic Data Based on Microwave Tomography (MWT) and Depth from EXtreme Points (DEXP) 

Francesco Mercogliano, Andrea Barone, Giusppe Esposito, Raffaele Castaldo, Pietro Tizzani, and Ilaria Catapano

In geophysics, it is common to employ multiple complementary geophysical exploration techniques to gather as much information as possible about the subsurface. In this framework, the concept of “data integration” emerges, referring to the combination of different datasets to extract more insights than those derivable from individual datasets alone, thereby enhancing information content and reducing interpretative ambiguities. While the goal of data integration is widely recognized, defining an optimal approach for the effective combination of different datasets remains an open research topic, strongly dependent on the acquired data and on the geophysical techniques considered.

In this work, we present a preliminary workflow for the integration of data from two main geophysical exploration techniques: Ground Penetrating Radar (GPR) and magnetic method. GPR is an active method sensitive to dielectric permittivity contrasts, while magnetic method is passive and sensitive to magnetic susceptibility contrasts. These two methods, despite being fundamentally different, are often used together in several contexts, enabling the detection and localization of buried targets through the analysis of electromagnetic and magnetic anomalies within the investigated domain.

Moreover, both methods benefit from advanced imaging techniques, such as Microwave Tomography (MWT) for GPR and Depth from EXtreme Points (DEXP) for magnetic data, which further enhance their potential in detecting and localizing anomalous bodies.

Specifically, the proposed workflow aims at the quantitative integration of GPR and magnetic data exploiting the results obtained from their respective MWT and DEXP imaging techniques, yielding a single composite result, which enhances interpretability and improves the characterization of anomalous targets in terms of morphology, position, and depth.

The workflow was validated through its application to simulated GPR and magnetic datasets for a common representative scenario, as well as to real datasets. Both simulated and real GPR and magnetic data were processed via MWT and DEXP, respectively, and subsequently their arithmetic integration was performed. The obtained results demonstrate the potential of the proposed workflow in obtaining a single result that outperforms the ones from individual methods, overcoming their limitations and yielding more accurate and detailed subsurface models.

Acknowledgments. This research has been founded by EU - Next Generation EU Mission 4, Component 2 - CUP B53C22002150006 - Project IR0000032 – ITINERIS - Italian Integrated Environmental Research Infrastructures System.

How to cite: Mercogliano, F., Barone, A., Esposito, G., Castaldo, R., Tizzani, P., and Catapano, I.: Arithmetic Integration of GPR and Magnetic Data Based on Microwave Tomography (MWT) and Depth from EXtreme Points (DEXP), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19830, https://doi.org/10.5194/egusphere-egu26-19830, 2026.

EGU26-19930 | Posters on site | GI1.1

Multi-scale and multi-sensor UAS-based approach for Geo-Agro-Environmental and Geophysical applications: the GAIA iLAB experience. 

Susi Pepe, Maurizio Buonanno, Andrea Barone, Andrea Vitale, Filippo Accomando, Raffaele Castaldo, Alessandra Iannuzzi, Francesco Mercogliano, Antonello Bonfante, and Pietro Tizzani

The integration of Unmanned Aerial Systems (UAS) into scientific research has established a crucial link between regional-scale satellite observations and high-resolution local-scale measurements. This study illustrates the operational framework and multi-disciplinary capabilities of GAIA iLAB (CNR), a laboratory designed to provide a structured guide for experimental activities in the geo-agro-environmental and geophysical sectors. By utilizing advanced technologies such as UAS, rovers, and in-situ acquisitions, GAIA iLAB addresses complex challenges ranging from precision agriculture to deep geophysical prospecting.

The laboratory manages a diverse UAS fleet, including DJI Matrice 300 RTK and Matrice 600 PRO platforms, which serve as versatile vectors for a wide array of specialized sensors. The research topics covered by GAIA iLAB are structured into four primary pillars of equal scientific priority:

  • Geophysics and Near-Surface Sensing: The lab conducts high-resolution magnetic and electromagnetic surveys. Utilizing drone-borne magnetometers (MagArrow) and vertical gradiometers (MagNimbus), the group investigates magnetization contrasts for archaeological research, geological-volcanological studies, and the search for buried structures. This is complemented by a Low-Frequency GPR system (Zond Aero LF) for urban geophysics and sub-surface investigations up to 10 meters deep.
  • Geo-Environmental Monitoring: Using LiDAR (DJI Zenmuse L1) and high-resolution RGB cameras, GAIA iLAB performs detailed topographic reconstructions (DSM/DTM) to monitor hydrogeological instability, landslide movements, and seismic-tectonic processes.
  • Advanced Agro-Environmental Research: The laboratory employs multispectral (Micasense Red-Edge M) and hyperspectral sensors (Senop HSC-2) to analyze vegetation health, crop water stress, and canopy temperature via thermal radiometric imaging (FLIR Vue Pro 640R).
  • Electromagnetic Induction (EMI): Focused on the "Near Surface Zone," the lab utilizes FDEM sensors (CMD Explorer 6L) to characterize soil apparent electrical conductivity (ECa) and resistivity, essential for understanding soil-atmosphere interactions and anthropogenic impacts.

The GAIA iLAB workflow ensures high-quality scientific output through rigorous flight planning (UgCS), strict adherence to EASA/ENAC regulations, and advanced data post-processing using SfM photogrammetry and LiDAR360 analysis. This integrated approach demonstrates the laboratory's potential to provide innovative solutions for environmental management and geophysical exploration.

How to cite: Pepe, S., Buonanno, M., Barone, A., Vitale, A., Accomando, F., Castaldo, R., Iannuzzi, A., Mercogliano, F., Bonfante, A., and Tizzani, P.: Multi-scale and multi-sensor UAS-based approach for Geo-Agro-Environmental and Geophysical applications: the GAIA iLAB experience., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19930, https://doi.org/10.5194/egusphere-egu26-19930, 2026.

EGU26-20018 | Posters on site | GI1.1

3D Thermo-Rheological Modelling of the Southern Apennines (Italy): Insights from the TRHAM Project 

Raffaele Castaldo, Maddalena Perrini, Filippo Accomando, Pietro Tizzani, Grazia De Landro, Gianluca Gola, Maurizio Fedi, Matteo Michele Cosimo Carafa, Vanja Kastelic, Deborah Di Naccio, Giuseppe Falcone, and Matteo Taroni

Southern Italy is a tectonically active region of major geodynamic significance, where long-lived convergence, post-collisional extension, slab rollback, and crust-mantle decoupling generate strong lateral and vertical heterogeneity in lithology, temperature, fluids, and deformation. Here, we present an integrated 3D Finite Element (FE) thermo-rheological model developed within the TRHAM project activities, aimed at reconstructing the regional thermal and mechanical architecture of the crust within a physically consistent, data-constrained framework. The FE geometry synthesizes a large body of published geological and geophysical constraints, integrating surface geology, regional structural interpretations, and deep wellbore information, complemented by gravity and magnetic evidence. The thermal field is computed under coupled conductive-convective regimes by solving the fully coupled Fourier heat-conduction and Darcy-flow equations in porous media. Boundary conditions include an altitude-dependent surface temperature, prescribed basal heat flow at Moho depth, and laterally adiabatic conditions. Key thermal parameters are calibrated through a bounded optimization strategy against independent thermal observables, while explicitly accounting for resolution limits and non-uniqueness. Rheological calculations combine a frictional failure criterion for brittle deformation and power-law creep for ductile flow, incorporating spatially variable pore-fluid pressure ratios derived from the thermo-hydraulic solution. Strain-rate scenarios are guided by regional geodetic strain-rate constraints and GNSS-informed kinematic parameters. The resulting strength envelopes and yield-stress distributions show strong spatial variations in effective crustal strength and in the depth and geometry of the BDT, both along the Apennine belt and from the Tyrrhenian side to the Adriatic foreland. The model highlights the mechanical impact of inherited crustal architecture and fluid-assisted weakening, and reproduces a systematic contrast between the Apulian foreland and the Apenninic wedge consistent with regional deformation and seismicity patterns. Explicit fluid flow further emphasizes how crustal geometry modulates hydraulic connectivity and hydrological decoupling between Apulian and Apenninic domains, focusing infiltration/discharge and shaping surface heat-flow patterns.

Acknowledgments

The activities are supported by the projects “Relation between 3D Thermo-Rheological Model and Seismic Hazard for Risk Mitigation in the Urban Areas of Southern Italy”, funded under the PRIN2022 PNRR initiative (code: P202299L2C), PRIN2022 PNRR, EU NextGenerationEU.

How to cite: Castaldo, R., Perrini, M., Accomando, F., Tizzani, P., De Landro, G., Gola, G., Fedi, M., Carafa, M. M. C., Kastelic, V., Di Naccio, D., Falcone, G., and Taroni, M.: 3D Thermo-Rheological Modelling of the Southern Apennines (Italy): Insights from the TRHAM Project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20018, https://doi.org/10.5194/egusphere-egu26-20018, 2026.

EGU26-20236 | Orals | GI1.1

Multiscale modelling of Magnetic field at Mefite D'Ansanto (Southern Apennines, Italy) 

Raffaele Castaldo, Andrea Barone, Filippo Accomando, Pietro Tizzani, Susi Pepe, Maurizio Buonanno, Francesco Mercogliano, Tony Alfredo Stabile, Antonio Napoliello, and Salvatore Grimaldi

The Mefite site in the Ansanto Valley (Southern Apennines, Italy) is a unique geological system characterized by intense low‑temperature gas emissions, primarily carbon dioxide (CO₂) and hydrogen sulfide (H₂S), emanating from a small sulfurous pond. Unlike typical geothermal or volcanic settings, these emissions occur in a non-volcanic environment and are associated with pseudo-volcanic processes linked to deposits formed during the Messinian salinity crisis. Mefite d’Ansanto is considered the largest natural source of low‑temperature CO₂-rich gases in a non‑volcanic setting on Earth, with an estimated daily emission of around 2000 tons. The gas discharge is supplied by a deep reservoir consisting of permeable limestone sequences overlain by low‑permeability clay layers, which help channel fluids toward the surface. In May 2025, we conducted a UAV‑based LiDAR survey followed by a magnetic survey to better characterize the subsurface structures guiding fluid flow in the Mefite area. The LiDAR dataset produced high‑resolution Digital Terrain (DTM) and Digital Surface Models (DSM) over 1.2 km², providing detailed topographic information essential for planning a terrain‑following magnetic survey with constant altitude relative to the ground. The UAV used for both LiDAR and magnetic acquisitions was a DJI Matrice 300 RTK. Magnetic data were collected using the Geometrics MagArrow magnetometer, equipped with Micro Fabricated Atomic Magnetometer (MFAM) sensors. These sensors have a sensitivity of 1 pT/√Hz and operate at a 1000 Hz sampling rate. MFAM technology is affected only by a polar dead zone, where the signal weakens when the sensor aligns within ±35° of the Earth’s magnetic field vector. A drone‑based magnetic surveys were performed on the main Mefite emission pond, was surveyed in May 2025, covering 350 × 450 m with 10 m line spacing; here, the MagArrow was suspended 3 m below the UAV. The surveys maintained an altitude of 35 m above ground level and a flight speed of 4 m/s. Magnetic data processing included corrections for heading errors and high-frequency rotor-induced noise, ensuring the isolation of true geophysical signals. The local geomagnetic parameters (declination 4°, inclination 57°) were used for reduction‑to‑the‑pole processing. The final magnetic map revealed an ellipsoidal anomaly (60–70 nT) centered on the CO₂ pond and a second, stronger anomaly northeast of the main vent. These anomalies are modelled to investigate the responsible source may related to magnetic minerals transported by deep fluids and precipitated near the emission vents.

Acknowledgments

The activities are partially supported by the projects “Relation between 3D Thermo-Rheological Model and Seismic Hazard for Risk Mitigation in the Urban Areas of Southern Italy”, funded under the PRIN2022 PNRR initiative (code: P202299L2C) and FRACTURES PRIN-MUR 2022 (grant no. 2022BEKFN2), both supported by the European Union-Next Generation EU.

How to cite: Castaldo, R., Barone, A., Accomando, F., Tizzani, P., Pepe, S., Buonanno, M., Mercogliano, F., Stabile, T. A., Napoliello, A., and Grimaldi, S.: Multiscale modelling of Magnetic field at Mefite D'Ansanto (Southern Apennines, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20236, https://doi.org/10.5194/egusphere-egu26-20236, 2026.

Shallow subsurface geology, often referred to as the critical zone, is fundamental to groundwater evaluation, aquifer recharge, environmental site investigations, and mining applications. Accurate characterization of this zone is required to identify infiltration pathways, low-permeability barriers, buried valleys, and channel structures, and to support decisions related to well placement, remediation, and resource management. Conventional methods such as electrical resistivity imaging (ERI) and ground conductivity meters are widely used but can be constrained by limited survey speed, discontinuous spatial coverage, sensitivity to near-surface disturbances, and logistical complexity in the field.

To overcome these limitations, a new transient electromagnetic (TEM) system, TEM2Go, has been developed for rapid, high-resolution shallow subsurface characterization. The system is optimized for depths from the surface to approximately 50–75 m while providing continuous lateral coverage along survey profiles. Acquisition speeds of 15–20 minutes per kilometre enable efficient mapping of large areas at high spatial density. A distinguishing feature of TEM2Go is real-time data processing and inversion, allowing near-instant visualization of subsurface conductivity during field operations. This enables adaptive survey design, where line spacing, follow-up measurements, and data density can be adjusted immediately based on observed results.

TEM2Go is the result of several years of research and development and incorporates multiple hardware innovations aimed at maximizing data quality while maintaining field practicality. The system design balances transmitter moment, receiver bandwidth, transmitter turn-off characteristics, and pulse repetition rates to achieve high resolution in the shallow subsurface. Both transmitter and receiver coils measure 65 × 65 cm and are designed for backpack-mounted operation. Each fully assembled unit weighs less than 12 kg, allowing deployment by a small field crew and enabling surveys in areas with limited or no vehicle access.

During data acquisition, the transmitter–receiver offset is continuously monitored, with a recommended operational offset of 15–20 m. This configuration supports continuous profiling while maintaining sufficient depth of investigation and resolution for near-surface applications. Real-time processing is fully integrated into the acquisition workflow. Recorded voltage decay curves are processed and inverted on-site, and conductivity models are displayed directly in the control software. Immediate access to inversion results improves quality control by revealing coupling effects, cultural noise, or offset inconsistencies as they occur, and provides rapid geological context to guide ongoing survey decisions.

The conference presentation describes the research and development process behind TEM2Go, highlighting key design choices and performance trade-offs. Case studies from collaboration with the Central Denmark Region are presented, where TEM2Go was used to map complex geology associated with point-source contamination. These examples demonstrate how rapid, high-resolution TEM profiling can improve identification of conductive pathways and geological controls on contaminant transport, supporting more targeted site characterization and remediation planning.

How to cite: Maurya, P. and Auken, E.: A lightweight small-loop TEM instrument for rapid near-surface mapping: Development and Case Studies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21366, https://doi.org/10.5194/egusphere-egu26-21366, 2026.

EGU26-21459 | ECS | Posters on site | GI1.1

Drone-based aeromagnetics combined with magnetotellurics to investigate volcanic structures at the Tajogaite volcano, La Palma Island. 

María C. Romero-Toribio, Fátima Martín-Hernández, Carlos Giménez-Berenguer, Perla Piña-Varas, Anna Martí, Alex Marcuello, Pilar Queralt, and Juanjo Ledo

Our regional aeromagnetic study of La Palma Island (Canary Islands), based on conventional airborne data, successfully imaged the island's large-scale magnetic structure. While the magnetic data provided a robust regional framework, they lacked the spatial resolution required to investigate shallow volcanic structures and post-eruptive thermal anomalies following the 2021 eruption. Therefore, a high-resolution, drone-based aeromagnetic survey was conducted over the Tajogaite volcano, targeting the area most affected by the eruption.

The survey was carried out in June 2024 and March 2025 using the DJI Matrice 210 RTK and DJI Matrice 300 RTK with a dual-sensor fluxgate magnetometer system sampling at 200 Hz. Constant-altitude flights covered an area of ~7 km2, with N-S-oriented survey lines spaced 30–60 m apart and tie lines spaced 150–200 m in the perpendicular direction. The drone flew in a lawnmower pattern, and we acquired high-altitude calibration flights in low magnetic gradient conditions to quantify and correct the magnetic measurements.

Data curation involved several processing stages, including removing inconsistent flight tracks and compensating for platform-induced noise using the calibration data. The total magnetic intensity map and anomaly were obtained by applying gridding and smoothing to the signal and then removing the IGRF model.

The resulting high-resolution magnetic anomaly map provides critical detail of the shallow magnetic structure of the Tajogaite volcanic edifice, allowing the identification of fault-controlled anomalies, low-susceptibility zones (after the 3D modelling of the data) related to high temperatures, and a potential shallow magma pathway.

Additionally, we acquired new magnetotelluric data along a North-South oriented profile, perpendicular to the inferred still-hot dyke direction. This enabled us to construct a 3D electrical resistivity model that correlates with the magnetic model to further analyse this area, which is likely to be related to the final stage of magma ascension.

This multidisciplinary research emphasises the importance of drone-based surveys in investigating active volcanic environments and post-eruptive dynamics on a local scale.

How to cite: Romero-Toribio, M. C., Martín-Hernández, F., Giménez-Berenguer, C., Piña-Varas, P., Martí, A., Marcuello, A., Queralt, P., and Ledo, J.: Drone-based aeromagnetics combined with magnetotellurics to investigate volcanic structures at the Tajogaite volcano, La Palma Island., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21459, https://doi.org/10.5194/egusphere-egu26-21459, 2026.

EGU26-21977 | Orals | GI1.1

Synthetic wind scenario generator from on-site SCADA for wind turbine digital twin 

Briac Malbois Le Borgne, Filippo Gatti, and Matteo Capaldo

Wind simulation is a critical step for wind turbine lifetime assessment: to accurately represent turbine behaviour across its lifespan, we need accurate wind scenarios. In this work, we propose a methodology for generating synthetic full-field turbulent wind scenarios from sparse, high-frequency SCADA (Supervision Control and Data Acquisition) collected across multiple wind farms.

The proposed methodology is a two-stage process. First, a physics-driven stochastic model learns wind data characteristics from low-frequency measurements extracted from high-frequency sparse SCADA. Second, the pipeline generates a low frequency signal that reproduces the observed spectral content, marginal distribution, and autocorrelation.

We build upon this first stage with a high-frequency turbulence generated via *PyConTurb* [1], which implements IEC/Kaimal coherence models to produce spatially coherent 3D velocity fields across the rotor plane. Our tool is first calibrated using learnt parameters from raw high-frequency SCADA data, then blended with the first signal, which is used as a constraint.

The pipeline outputs TurbSim-compatible BTS files [2] , enabling use in SeaHowl [3] aeroelastic simulations. This industry-standard output enables a ready-to-use wind scenario in both simulation pipelines and machine learning analysis tools.

[1] (Rinker, J. M. (2018). PyConTurb: an open-source constrained turbulence generator. _Journal of Physics: Conference Series_, _1037_, 062032. https://doi.org/10.1088/1742-6596/1037/6/062032) 
[2] (Jonkman, B J (2006). TurbSim User's Guide. https://doi.org/10.2172/891594) 
[3] (De Lataillade, T., Yu, W., Pallud, M., & Capaldo, M. (2024). SEAHOWL: Partitioned Multiphysics and Multifidelity Modelling of Wind Turbines with Monolithically Coupled Elastodynamics. _Journal of Physics: Conference Series_, _2767_(5), 052051. https://doi.org/10.1088/1742-6596/2767/5/052051) 

How to cite: Malbois Le Borgne, B., Gatti, F., and Capaldo, M.: Synthetic wind scenario generator from on-site SCADA for wind turbine digital twin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21977, https://doi.org/10.5194/egusphere-egu26-21977, 2026.

GI2 – Data networks and analysis

EGU26-304 | ECS | Orals | GI2.1

Detecting Fin Whale Calls from Ocean-Bottom Seismometer Data with Deep Learning 

Jocelyn Japnanto, Alex Saoulis, Miriam Romagosa, Rita Leitão, Mónica A. Silva, Matt Graham, and Ana M. G. Ferreira

Fin whales (Balaenoptera physalus) produce low-frequency vocalisations that propagate efficiently through the ocean and seafloor, making them detectable on broadband ocean bottom seismometers (OBS). While primarily deployed for seismic studies, OBSs offer a unique and cost-effective opportunity for passive acoustic monitoring (PAM) of marine mammals in remote regions over extended periods. Traditional detection and classification of whale calls have relied on energy thresholding, cross-correlation, or matched filtering techniques. These approaches, however, may falter in performance in high-noise environments typical of OBS datasets and often require extensive manual post-processing, making them a labour-intensive process. These limitations motivate automated, noise-robust approaches capable of exploiting the growing volume of seismic data now available.

We present a deep learning framework for detecting fin whale calls from broadband OBSs surrounding the São Jorge Island in the Azores, as well as up to twenty stations of the wider UPFLOW array spanning the Azores–Madeira–Canaries region. Our method uses a semantic segmentation model that operates on spectrogram representations between 12–35 Hz, a frequency band encompassing the classic ‘20-Hz’ fin whale note and the lower frequency ‘backbeat’. The model architecture includes a ResNet-18 encoder pretrained on ImageNet with a U-Net decoder to identify calls in both time and frequency. Training was conducted on a dataset comprising of ~6 days of manually annotated spectrograms and an additional ~6 days of background-only spectrograms. Performance was evaluated using mean Intersection-over-Union and F1-score, achieving 0.65 and 0.80 respectively.

Once validated, the model was applied to months- to year-long OBS records across the region. Fin whale calls were detected at all stations, with clear seasonal patterns showing peak calling activity between October and February, consistent with known migratory patterns in the North Atlantic. Spatial differences in call characteristics and temporal patterns further revealed potential regional variations in vocal behaviour, offering insights into song plasticity and complexity.

By applying a deep learning-based detector on OBS data, we show that machine learning provides a powerful and efficient approach to automating fin whale call detection at scale. Our method processed hundreds of thousands of hours of OBS recordings and identified nearly a million calls across all stations. This large-scale detection unlocks detailed analyses of vocal behaviour, spatial distribution, and seasonal trends, deepening our understanding of their behaviour in the north-east Atlantic. Our findings not only highlight the interdisciplinary value of OBS datasets, but also the potential of machine learning in supporting PAM efforts for the conservation and management of wide-ranging marine species.

How to cite: Japnanto, J., Saoulis, A., Romagosa, M., Leitão, R., Silva, M. A., Graham, M., and Ferreira, A. M. G.: Detecting Fin Whale Calls from Ocean-Bottom Seismometer Data with Deep Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-304, https://doi.org/10.5194/egusphere-egu26-304, 2026.

EGU26-716 * | ECS | Orals | GI2.1 | Highlight

An Integrated Digital Framework for Multi-Scale Water Security in Africa. 

Samuel Berchie Morfo and Nana Kwame Osei Bamfo

This presentation outlines a comprehensive framework of multi-scale digital solutions designed to address Africa's pressing water challenges. We explore the integration of advanced physical modelling with a diverse suite of next-generation hydrologic observations from remote sensing and in-situ networks to crowd-sourced data. The core of our approach lies in automated systems for data fusion, processing, and assimilation, leveraging machine learning and hybrid techniques to enhance model accuracy. Critically, we incorporate robust uncertainty quantification to ensure reliable outputs. These integrated components enable the development of actionable, real-time forecasting and decision support systems for water resources allocation and disaster management. We will demonstrate practical applications, including autonomous processes and embedded devices, showcasing a transformative pathway towards proactive, data-driven water governance across the African continent.

How to cite: Berchie Morfo, S. and Bamfo, N. K. O.: An Integrated Digital Framework for Multi-Scale Water Security in Africa., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-716, https://doi.org/10.5194/egusphere-egu26-716, 2026.

The Gross Calorific Value (GCV) indicates coal quality by measuring the total heat released during the complete combustion of the coal. Accurate GCV estimation is crucial for efficient pricing, processing, and energy performance assessment in industries. Conventional oxygen bomb calorimetry, though precise, is relatively slow and expensive for large-scale analyses. Since coal’s organic and elemental composition strongly affects its heating value, understanding this relationship can help with reliable GCV evaluation. In this study, we analyzed the mid-infrared FTIR spectra of coal and selected 56 absorption bands associated with the relevant organic and elemental constituents of coal. These were used as input features for various machine learning (ML) models to predict the GCV of coal from the Johilla coal basin in India. The ML models tested included piecewise linear regression (PLR), partial least squares regression (PLSR), support vector regression (SVR), random forest regression (RFR), artificial neural networks (ANN), and extreme gradient boosting regression (XGB). By combining the predictions from the three models (PLSR, RFR, and XGB) through a simple average, we achieved the highest accuracy (R² = 0.951, RMSE = 19.05%, MBE = 1.42%, MAE = 4.053 cal/g), indicating strong agreement between the predicted and measured values. Overall, the FTIR-based method yields results that match or surpass those of traditional laboratory techniques reported in earlier research. The GCV values predicted from the FTIR models were statistically tested using t-tests (test for mean) and F-tests (test for variance) at a 1% significance level and were found to be statistically similar to the results from the standard bomb calorimeter method. The study demonstrates that the FTIR-based approach is independent and reliable and can be used as a faster and more convenient alternative method for determining GCV, making it highly useful for quick coal quality analysis in industry.

How to cite: Vinod, A., Prasad, A. K., and Varma, A. K.: A novel method for rapid and reliable estimation of Gross Calorific Value (GCV) of Coal using mid-infrared FTIR Spectroscopy and a multi-model Machine Learning Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1075, https://doi.org/10.5194/egusphere-egu26-1075, 2026.

EGU26-1760 | ECS | Orals | GI2.1

Toward Robust Three-Dimensional Magnetic and Gravity Inversion Using Deep Learning 

Shiva Tirdad, Gilles Bellefleur, Fidele Yrro, Mojtaba Bavand Savadkoohi, and Erwan Gloaguen

Magnetic and gravity surveys remain among the most cost-effective geophysical tools for investigating the subsurface. They provide information on rock geometry and bulk properties at regional to deposit scale, and they have long been used to guide mineral exploration. However, turning geophysical anomalies into reliable three-dimensional property models requires inversion, a process that is inherently non-unique: multiple subsurface distributions can explain the same anomaly. Conventional approaches, such as least-squares or Bayesian inversion, can produce valuable results; however, they remain computationally demanding for large 3D models and require strong regularization choices that may bias geological interpretation.
Over the last decade, geoscientists have explored machine learning as an alternative approach. Instead of repeatedly solving forward equations, machine learning methods learn a mapping between geophysical anomalies and subsurface properties using large training libraries of synthetic examples. Early work with convolutional neural networks (CNNs) and U-Net architectures showed the concept is viable for electromagnetic and seismic data. More recent studies have shown that deep neural networks can recover magnetic susceptibility distributions from magnetic data and, in some cases, perform joint inversion of gravity and magnetic observations. Nevertheless, purely convolutional architectures often struggle to preserve long-range spatial relationships in fully three-dimensional volumes, resulting in blurred boundaries and reduced geological interpretability.
Recent advances in deep learning offer new opportunities to address these limitations. Emerging models are designed to capture long-range dependencies and preserve sharper boundaries. They have been effective in other 3D volumetric fields, such as medical imaging and seismic interpretation, but have yet to be explored for potential-field inversion.
In this study, we develop a deep-learning-based inversion method for magnetic and gravity data aimed at critical mineral exploration. The approach targets mineral systems with distinct geophysical signatures, with a focus on volcanogenic massive sulfide (VMS) environments. By combining data-driven learning with physics-informed training, the method produces reproducible three-dimensional susceptibility and density models that reduce ambiguity in subsurface interpretation. The workflow is tested using data from the Flin Flon VMS district in Manitoba, Canada, demonstrating its potential to improve targeting of buried copper-zinc mineralization and to support the integration of advanced AI methods into geoscience workflows.

 

How to cite: Tirdad, S., Bellefleur, G., Yrro, F., Bavand Savadkoohi, M., and Gloaguen, E.: Toward Robust Three-Dimensional Magnetic and Gravity Inversion Using Deep Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1760, https://doi.org/10.5194/egusphere-egu26-1760, 2026.

EGU26-3405 | Orals | GI2.1

SatWellMCQ: A Vision–Language Satellite Datasetfor MCQ-Based Image Grounding of Oil Wells 

Ahmed Emam, Sultan Alrowili, Mathan K. Eswaran, Romeo Kinzler, and Younes Samih

Monitoring oil and gas wells is essential for assessing environmental degradation and long-term impacts such as methane emissions from abandoned and orphaned wells. Satellite imagery combined with machine learning offers scalable capabilities for detecting and characterizing oil and gas infrastructure, yet progress remains constrained by the lack of multimodal, multiple-choice (MCQ) vision-language datasets that enable structured evaluation and post-training of vision-language models (VLMs) for oil well scene grounding. Existing resources are predominantly visual-only and therefore provide limited support for image grounding from satellite imagery.

To address this gap, we introduce SatWellMCQ, a vision-language dataset of expert-verified satellite imagery paired with natural-language descriptions and multiple-choice supervision for image-grounded identification and localization of oil wells. SatWellMCQ uses high-resolution multispectral Planet imagery (RGB and infrared) and text annotations that describe well type and spatial context. Each sample includes one expert-verified correct description and three semantically plausible distractor descriptions drawn from other samples, enabling structured MCQ evaluation. All samples were manually verified by a senior domain expert with 100% intra-expert agreement, ensuring accurate alignment between images, labels, and text. The dataset covers four categories relevant to oil well monitoring: active wells, suspended wells, abandoned wells, and control samples without visible wells, yielding a balanced distribution for training and evaluation. We publicly release SatWellMCQ to support research on image grounding and vision-language adaptation in satellite imagery of oil wells.

We evaluate SatWellMCQ across state-of-the-art VLMs in zero-shot and supervised fine-tuning (SFT) settings. In the zero-shot setup, performance is moderate only for large-scale models, with the best result achieved by Qwen3-VL-235B at 0.670 accuracy. Compact models transfer poorly in zero-shot evaluation (e.g., Granite~3.3~2B at 0.422 and Phi-4-multimodal-instruct~6B at 0.376), highlighting the difficulty of domain-specific oil well analysis without targeted supervision. Supervised fine-tuning on SatWellMCQ yields substantial gains for compact models: Granite~3.3~2B improves to 0.722 and Phi-4-multimodal-instruct~6B reaches 0.730, surpassing all zero-shot baselines. These results show that SatWellMCQ poses a challenging benchmark for current VLMs while enabling effective domain adaptation through structured MCQ supervision.

Overall, SatWellMCQ provides a resource for post-training and benchmarking VLMs on image grounding of oil wells in satellite imagery and supports  geoscientific monitoring tasks relevant to environmental impact assessment and methane mitigation.

How to cite: Emam, A., Alrowili, S., Eswaran, M. K., Kinzler, R., and Samih, Y.: SatWellMCQ: A Vision–Language Satellite Datasetfor MCQ-Based Image Grounding of Oil Wells, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3405, https://doi.org/10.5194/egusphere-egu26-3405, 2026.

EGU26-4011 | ECS | Orals | GI2.1

Identifying valuable forest habitats for conservation in north-western Germany using AI and citizen science 

Katharina Horn, Daniele Silvestro, Christine Wallis, Pedro J. Leitao, Ender Daldaban, and Annette Rudolph

Around the globe we experience a significant biodiversity loss, mainly driven by direct anthropogenic exploitation, land use changes, and climate change. The most effective strategy to limit biodiversity loss is the designation and management of protected areas. Consequently, the European Union has adopted the EU Biodiversity Strategy for 2030, aiming to protect 30% of aquatic and terrestrial ecosystems by 2030. However, a consistent framework to designate protected areas across all EU member states is lacking. Additionally, the monitoring of biodiversity is challenged by the dynamic nature of the biological system, exacerbated by ongoing climate change, putting additional pressure on the member states in the identification of suitable areas for conservation. 

In contrast, the increasing amount of detailed geospatial and climatic data contains valuable information that can be used to optimise protected area designation. Recent developments in artificial intelligence and machine learning now provide us with powerful tools to best utilise these vast amounts of data. In this study, we develop a transparent and reproducible framework to prioritise protected areas in forests. Here we apply the CAPTAIN framework based on reinforcement learning (RL) to identify valuable forest habitats for conservation in the federal state of North Rhine-Westphalia (NRW), Germany. First, we model habitats of ten forest bird indicator species across the period of 2016-2024. Second, we use the changing habitat patterns to train a RL model that identifies 30% of the most valuable forest sites in the federal state. Finally, we model valuable forest sites under different policies (e.g., including or excluding opportunity costs for nature conservation) to illustrate how potential limitations of nature conservation management can be addressed. Our results indicate that forest sites in the south-east of NRW are most suitable for conservation. Furthermore, we find that including opportunity costs for nature conservation in the model predictions produces similarly strong outcomes for safeguarding the most endangered bird species. The framework makes use of open-source data and can be applied to any other region or country to support strategic nature conservation management.

How to cite: Horn, K., Silvestro, D., Wallis, C., Leitao, P. J., Daldaban, E., and Rudolph, A.: Identifying valuable forest habitats for conservation in north-western Germany using AI and citizen science, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4011, https://doi.org/10.5194/egusphere-egu26-4011, 2026.

Geological mapping in complex metallogenic provinces often relies on band ratios and thresholding techniques. While effective for simple targets, these traditional methods struggle to capture non-linear spectral associations inherent in natural mineral mixtures and require significant prior knowledge of the target mineralogy. This study introduces a novel, data-driven unsupervised pipeline for mineral target generation, applied to the Aït Saoun region in the Moroccan Anti-Atlas, a strategic zone characterized by polymetallic occurrences (Cu, Co, Fe, Mn).

We leverage the full spectral topology of ASTER satellite imagery (VNIR-SWIR bands) rather than reduced indices. Our approach integrates topological manifold learning to reduce the high-dimensional spectral space, followed by density-based spatial clustering to delineate mineral clusters. This combination allows for the preservation of local data structure and the automated rejection of noise without human supervision.

The pipeline successfully identified spatially coherent clusters corresponding to specific hydrothermal alteration zones. It autonomously distinguished between structural iron-manganese anomalies and lithology-controlled copper mineralization a nuance often missed by standard linear ratios. The metallogenic relevance of these spectral clusters was rigorously validated through field mapping and geochemical analysis using Atomic Absorption Spectroscopy (AAS). Results confirmed economic grades in the predicted zones, yielding Copper concentrations up to 2.60% in propylitic alteration zones and Iron-Manganese oxide grades (21.94% Fe, 1.80% Mn) in tectonic corridors. Furthermore, the detection of distal barite anomalies highlights the method’s capability to map complete hydrothermal zonations.

These findings demonstrate that topological machine learning offers a robust, superior alternative to conventional remote sensing techniques for vectoring exploration targets in arid environments. By converting raw spectral data into validated metallogenic maps, this pipeline provides a scalable tool for de-risking early-stage mineral exploration in the Anti-Atlas.

How to cite: Elomairi, M. A. and El GAROUANI, A.: Automated Mineral Cluster Detection in ASTER Data Using Topological Machine Learning: A Novel Data-Driven Approach for Geological Exploration in Ait Saoun, Anti Atlas, Morocco, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4179, https://doi.org/10.5194/egusphere-egu26-4179, 2026.

EGU26-4956 | ECS | Posters on site | GI2.1

Electromagnetic & Cone Penetration Test Data Fusion on Soil Characterization 

Dimitrios Madelis, Marios Karaoulis, and Philippe De Smedt

Defining subsurface soil conditions in complex coastal settings requires the use of both geophysical and geotechnical datasets, each with different resolution and sensitivity. This study combined helicopter-borne electromagnetic (HEM) data, where large areas are spatially covered with limitations to vertical resolution, with cone penetration test (CPT) data, where high resolution can be achieved while the spatial resolution often is very sparse due to drilling associated costs. Τo formulate a continuous three-dimensional model of subsurface soil properties for levee risk assessment, these datasets were integrated. HEM data provides extensive covering resistivity profiles, while CPT provides high resolution, spatially limited measurements of mechanical soil behaviour.
It is known that resistivity as a soil property depends on many parameters (mostly water quality and soil type), and there is no straightforward method to directly translate it to soil, hence the use of ML. To deal with these complexities, we employed machine learning methods – Random Forests and neural networks – to merge heterogeneous datasets and predict continuous soil behaviour indices and discrete lithological types. We propose the use of multiple features, such as spatial coordinates, depths, distance from coast, soil types and local geological conditions. After pre-processing, machine-learning models were trained to fuse the datasets to ensure spatial consistency in the coastal environment. Afterwards, the Soil Behaviour Type Index (SBT) (Robertson, 1990) was calculated using the CPT measurements and then was discretized into lithological units.
A classical machine learning algorithm (Random Forest) and a PyTorch-based neural network were trained for regression (predicting the continuous SBT index) and classification (predicting soil types) tasks, and their performance was evaluated using standard statistical and visual metrics. Final models were retrained on the full dataset to increase generalizability and robustness. The final product is to map 𝐼𝑐 values and lithological classes at every HEM point and ultimately to make a 3D subsurface soil model. The outcome for each process was validated against an 80%-20% test to ensure reasonable results.
While regression models had similar RMSE scores, classification models generally produced models with greater accuracy of dominant soil types but captured fewer underrepresented mixed lithologies. This work focuses on the interpretability of soil models through integrating data (i.e., not just purely statistical but spatial output) and ultimately continuity in the spatial domain (where engineers are most concerned). The goal of this study is to develop a framework where continuous geophysical data, collected either by helicopters or drones can be combined with additional geological boreholes and CPTs and other geotechnical information, to enable us to image the subsurface beyond resistivity. One of the products of this study serves to represent an approach to providing a better product to those grappling with levee design and safety.

How to cite: Madelis, D., Karaoulis, M., and De Smedt, P.: Electromagnetic & Cone Penetration Test Data Fusion on Soil Characterization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4956, https://doi.org/10.5194/egusphere-egu26-4956, 2026.

EGU26-5687 | ECS | Orals | GI2.1

Application of Gaussian Mixture Models for Geochemical Anomaly Detection 

Judith Jaeger, José I. Barquero, Julio A. López-Gómez, and Pablo Higueras

Geochemical prospecting is a fundamental tool in mineral exploration. Traditionally, the interpretation of geochemical data has relied on classical statistical methods, which in many cases are univariate or linear in nature and may fail to adequately capture the complex multivariate relationships among geochemical parameters. In this context, machine learning approaches offer an alternative framework for the integrated analysis of multivariate data and the identification of hidden patterns. 

This study evaluates the application of a Gaussian Mixture Model (GMM) as an unsupervised method for the identification of geochemical anomalies of potential geological interest. The analysis was conducted on a dataset of 114 soil samples collected from the southwestern sector of the province of Ciudad Real. Before the application of the GMM, an exploratory statistical analysis was performed, including the Kaiser–Meyer–Olkin (KMO) test and the Measure of Sampling Adequacy (MSA), aimed to assess the suitability of the variables for multivariate analysis. 

After conducting several experiments, the results indicate that the Gaussian Mixture Model can identify zones with anomalous values consistent with geological interest, highlighting its potential as a supportive tool in geochemical prospecting. 

How to cite: Jaeger, J., Barquero, J. I., López-Gómez, J. A., and Higueras, P.: Application of Gaussian Mixture Models for Geochemical Anomaly Detection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5687, https://doi.org/10.5194/egusphere-egu26-5687, 2026.

EGU26-6107 | ECS | Posters on site | GI2.1

Forecasting Offshore Caisson Tilt via Deep Learning: A Numerical Simulation-Based Approach Accounting for Geotechnical Uncertainty 

Saeyon Kim, Jingi Hong, Inyoung Huh, and Heejung Youn

This study presents a comparative analysis of time-series forecasting models to predict caisson tilt using early-stage monitoring data. To establish a training dataset that accounts for inherent geotechnical uncertainty, 1,000 2D numerical simulations were performed using PLAXIS2D, based on an actual design case in South Korea. To incorporate spatial variability, the subsurface was discretized into 61 independent zones: Deep Cement Mixing (33 zones), foundation rubble (6 zones), backfill rubble (10 zones), and underlying heaving soil (12 zones). Geotechnical parameters including elastic modulus (E), undrained shear strength (Su), and interface strength reduction factor (Rinter), were varied by up to 50% of their design values. Latin Hypercube Sampling (LHS) was used to assign geotechnical properties to each zone. Each case simulated a 28-stage construction sequence, with caisson tilt extracted at each stage to generate time-series data.

Four forecasting models such as ARIMA, LSTM, Temporal Convolutional Network (TCN), and an encoder-only Transformer, were evaluated. The dataset was split into 680 simulations for training, 170 for validation, and 150 for testing. Forecasting performance was assessed across varying initial observation lengths (cut = 3, 5, 10, 15, and 20 stages) to predict all remaining future stages. Results indicate that while the statistical baseline (ARIMA) showed consistently high errors regardless of observation length, with RMSE values of approximately 0.09 at cut = 3 and 0.08 at cut = 10. In contrast, deep learning models exhibited clear error reductions as more initial observations became available. Among the tested models, the TCN achieved the highest accuracy, with RMSE values of approximately 0.006 at cut = 10 and 0.004 at cut = 15. The encoder-only Transformer model also maintained stable performance for cut ≥ 10, with RMSE values below 0.01.

Acknowledgements This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2023R1A2C1007635).

How to cite: Kim, S., Hong, J., Huh, I., and Youn, H.: Forecasting Offshore Caisson Tilt via Deep Learning: A Numerical Simulation-Based Approach Accounting for Geotechnical Uncertainty, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6107, https://doi.org/10.5194/egusphere-egu26-6107, 2026.

EGU26-6766 | ECS | Posters on site | GI2.1

Rapid Bayesian Geophysical Inversion Using General Geophysical Neural Operator 

heng zhang and yixian xu

Bayesian inversion provides a rigorous framework for uncertainty quantification in geophysics, but is often computationally prohibitive due to the reliance on Markov Chain Monte Carlo (MCMC) sampling, which requires massive numbers of forward simulations. While deep learning surrogate models offer acceleration, existing architectures (e.g., CNNs, FNO, DeepONet) often struggle with fixed discretization constraints and cannot flexibly handle the irregular observation coordinates typical in field surveys.

To address these challenges, we propose the General Geophysical Neural Operator (GGNO), a novel Transformer-based architecture designed for mesh-independent operator learning. This design fulfills three fundamental requirements for forward solvers in the context of practical inversion: (1) Discretization-invariant, allowing the processing of input models with different mesh resolutions; (2) Prediction-free, enabling direct solution querying at arbitrary spatio-temporal coordinates; and (3) Domain-independent, decoupling input and output discretizations. 

We validate GGNO on Magnetotelluric (MT) forward modeling, demonstrating exceptional generalization while achieving accuracy two orders of magnitude higher than traditional methods. By integrating GGNO into a Bayesian framework, we achieve highly efficient MCMC sampling, reducing the computational time from tens of days to a few minutes, which allows for a comprehensive exploration of the posterior distribution. Applied to field data, this approach successfully recovers complex subsurface resistivity structures with rigorous uncertainty bounds. These results highlight GGNO's potential to enable high-precision subsurface imaging and robust probabilistic interpretation for complex geophysical exploration.

How to cite: zhang, H. and xu, Y.: Rapid Bayesian Geophysical Inversion Using General Geophysical Neural Operator, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6766, https://doi.org/10.5194/egusphere-egu26-6766, 2026.

EGU26-7774 | ECS | Posters on site | GI2.1

Probabilistic Reconstruction of Sentinel-2 Satellite Image Time Series Using Multi-Sensor Gaussian Process Models 

Bastien Nespoulous, Alexandre Constantin, Dawa Derksen, and Veronique Defonte

Satellite Image Time Series (SITS) are a cornerstone of Earth observation, enabling long-term monitoring of environmental processes such as vegetation dynamics, land-use change, and natural hazards. However, optical satellite time series, including Sentinel-2, are frequently irregular and incomplete due to cloud cover, atmospheric effects, and acquisition constraints, which strongly limit their usability in operational monitoring systems. In contrast, Sentinel-1 Synthetic Aperture Radar (SAR) provides regular observations for any weather condition and offers complementary information for mitigating optical sensor limitations. Generating dense and reliable Sentinel-2 time series from multi-sensor observations therefore remains a critical challenge.

This work investigates Gaussian Process (GP) based statistical models for the reconstruction and densification of Sentinel-2 image time series by jointly exploiting Sentinel-1 and Sentinel-2 data. Gaussian Processes offer a flexible Bayesian framework for pixel interpolation and extrapolation. We explore GP formulations capable of handling irregular temporal sampling, multi-output dependencies, and latent variable structures, enabling the fusion of heterogeneous optical and radar observations.

An in-depth analysis of the state-of-the-art is conducted, covering multi-output Gaussian Processes, sparse and variational approximations for scalability, latent variable models (including hierarchical GP-LVMs), and inverse GP approaches based on shared latent spaces. These methods are evaluated with respect to three key challenges: ensuring spatio-temporal coherence of reconstructed images, fusing asynchronous multi-sensor observations, and maintaining computational tractability for large-scale satellite datasets.

To support experimental investigations, a representative multi-regional dataset is constructed over mainland France and overseas territories, capturing diverse climatic patterns, land-cover types, and cloud conditions, including extreme events such as flooding. 

This study establishes the methodological foundations for reconstructing dense Sentinel-2 time series conditioned on Sentinel-1 observations, with explicit uncertainty quantification. By leveraging Sentinel-1 data, the approach effectively imputes missing Sentinel-2 values while providing consistent average pixel estimates with associated uncertainty, which is critical for geoscience applications. The proposed framework contributes toward more robust Earth observation monitoring systems and the development of reliable geospatial digital twins.

How to cite: Nespoulous, B., Constantin, A., Derksen, D., and Defonte, V.: Probabilistic Reconstruction of Sentinel-2 Satellite Image Time Series Using Multi-Sensor Gaussian Process Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7774, https://doi.org/10.5194/egusphere-egu26-7774, 2026.

EGU26-7860 | Posters on site | GI2.1

Densification and forecasting of Sentinel-2 time series from multimodal SAR and optical satellite data using deep generative models 

Véronique Defonte, Dawa Derksen, Alexandre Constantin, and Bastien Nespoulous

Sentinel-2 optical image time series are a key source of information for many Earth observation applications, including climate monitoring, agriculture, ecosystem dynamics, and land surface change analysis. Dense and regular observations are essential to accurately capture seasonal patterns, abrupt events, and long-term trends. However, in practice, Sentinel-2 time series are often sparse and irregular due to cloud cover and varying acquisition conditions. These limitations significantly complicate continuous monitoring and the analysis of surface dynamics. Moreover, beyond time series densification, there is a growing need to anticipate future optical observations to support scenario analysis, early warning systems, and predictive environmental monitoring.

To address these challenges, we propose a deep learning–based framework for densifying Sentinel-2 time series by generating plausible optical images at arbitrary past or future dates. The approach relies on multimodal satellite observations, jointly exploiting optical Sentinel-2 and radar Sentinel-1 data. Indeed, SAR measurements are insensitive to cloud cover and provide complementary structural and temporal information. This multimodal setting enables the reconstruction of missing observations and the prediction of future optical states while preserving realistic spatio-temporal dynamics.

From a methodological perspective, the model is explicitly designed to handle sparse, incomplete, and temporally misaligned multimodal time series. It operates on temporal sets of Sentinel-2 and Sentinel-1 images acquired at irregular dates around a target time. A cross-attention mechanism is used to explicitly model interactions across time and modalities, allowing the network to identify and weight the most relevant observations for generating a Sentinel-2 image at a given target date.

In addition, the proposed framework incorporates a probabilistic decoder that estimates not only the predicted Sentinel-2 image but also an associated uncertainty map. This uncertainty estimation provides valuable insight into the confidence of the generated pixels, which is particularly important for downstream applications such as anomaly detection, risk assessment, and decision-making support.

The model is evaluated across multiple geographical regions and land-cover types, demonstrating strong performance in both densification and forecasting tasks. Results show that the proposed approach successfully preserves the temporal dynamics of the scenes, notably by accurately reproducing vegetation phenology as reflected in NDVI time series. Forecasting experiments further highlight the importance of radar information: Sentinel-1 observations close to the target date allow the model to detect surface changes occurring after the last available optical image, thereby improving future predictions. Overall, the proposed method represents a step towards the densification and forecasting of Sentinel-2 time series, offering a promising direction for future methodologies aimed at continuous Earth surface monitoring and predictive analysis.

How to cite: Defonte, V., Derksen, D., Constantin, A., and Nespoulous, B.: Densification and forecasting of Sentinel-2 time series from multimodal SAR and optical satellite data using deep generative models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7860, https://doi.org/10.5194/egusphere-egu26-7860, 2026.

EGU26-8542 | Orals | GI2.1

A Big Data and Text Mining–Based Media Analysis Framework for Disaster Cause Investigation 

Jin Eun Kim, Heeyoung Shin, and Sengyong Choi

 As similar disasters and accidents continue to occur, public concern about the limitations of existing disaster response systems and the need for institutional improvement is increasing. The National Disaster Management Research Institute of Korea conducts disaster cause investigations as part of its statutory responsibilities, examining problems observed before and after disasters, institutional weaknesses, and public demands for improvement. In this context, news data provide valuable unstructured information that reflects on-site conditions, response activities, policy debates, and public opinion, and thus complement official investigation records in understanding institutional and managerial factors related to disasters.


 This study aims to develop a media analysis framework based on big data and text mining for use in disaster cause investigations. Disaster-related news articles were first collected, and a large language model (Gemini) was applied to identify and extract sentences that describe problems and suggested improvements in the stages of disaster occurrence and response. The extracted sentences were then processed using natural language processing techniques, including stopword removal and the merging of duplicate and semantically similar sentences. Based on semantic similarity, the remaining sentences were grouped to organize major issues. In addition, nouns were extracted and their frequencies were analyzed by year to identify key terms and to examine changes in topics emphasized in media coverage.
 

 Applying the proposed framework to the disaster cause investigation of the 2023 Osong Underpass Flooding Disaster conducted in 2025, we identified 21 problem items grouped into seven categories, such as insufficient pre-closure of the underpass and inadequate maintenance of river embankments. In addition, 17 improvement measures were derived in six categories, including improvements to underpass closure criteria and flood risk grading, as well as the strengthening of river management practices, and were systematically organized and proposed. The results indicate that combining news big data, text mining, and large language models can effectively structure key issues and institutional weaknesses, and can serve as a useful analytical tool for strengthening the evidence base and explanatory power of disaster cause investigations.

How to cite: Kim, J. E., Shin, H., and Choi, S.: A Big Data and Text Mining–Based Media Analysis Framework for Disaster Cause Investigation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8542, https://doi.org/10.5194/egusphere-egu26-8542, 2026.

EGU26-10174 | ECS | Orals | GI2.1

A global–hierarchical–categorical alignment framework to address sample scarcity and domain shift in crop mapping 

Jingya Yang, Qiong Hu, Mariana Belgiu, and Wenbin Wu

The scarcity and high acquisition cost of field crop samples remain a major bottleneck for applying Artificial Intelligence (AI)–driven supervised learning methods in large-scale geoscientific applications such as crop type mapping. Meanwhile, crop phenology and, consequently, spectra-temporal characteristics of the same crop type present significant interannual and regional variations due to the differences in local conditions and human activities, such as climatic, soil properties and farming practices. This causes the “domain shift” challenge. Therefore, directly applying a classification model trained in a specific region and year to a new region or year inevitably leads to poor prediction performance. The gap between the abundant availability of Earth Observations imagery and the limited accessibility of training crop samples hider efficient mapping of varied crop types across large regions. To address training sample scarcity and cross-region/year domain shift in large-scale crop type mapping, we propose a transferable crop mapping method named Global-Hierarchical-Categorical feature Alignment (GHCA). GHCA integrates unsupervised domain adaptation, contrastive learning, and pseudo-labeling to achieve multi-dimensional alignment between source domain and target domain at global, hierarchical and categorical levels. The developed method enables accurate and transferable crop mapping across diverse agricultural landscapes with minimum field survey requirements. The main contributions of our study can be summarized as follows: (1) A global feature pre-alignment mechanism is introduced by calculating the Multi-Kernel Maximum Mean Discrepancy (MK-MMD) metric across different hierarchical features to align source and target domains in global and hierarchical feature spaces. This mechanism substantially improves the initial reliability of pseudo-labels generated for the target domain, providing a reliable foundation for subsequent fine-grained categorical level feature alignment; (2) A robust pseudo-label generation strategy is developed by jointly considering prediction confidence, prediction certainty, and prediction stability. Reliable pseudo-labels for target domain are selected by calculating model prediction probabilities and predictive uncertainty estimates through teacher-student model. Moreover, the Exponential Moving Average (EMA) strategy is adopted to updated model parameters in the teacher path to enable the acquisition of obtaining more stable pseudo-labels; (3) Category-wise feature alignment is achieved by integrating pseudo-labeling with contrastive learning, which explicitly pulls intra-class feature closer for the same crop types across source and target domains, while pushing inter-class feature apart for different crop types. The effectiveness of the proposed GHCA method for both cross-region and cross-year crop mapping was evaluated across five regions in China and the U.S. over a two-year timeframe. GHCA was compared with a machine learning method (RF), supervised deep learning models (DCM, Transformer, and PhenoCropNet), and transfer learning methods (DACCN, PAN, and CSTN) for cross‑year and cross‑region crop mapping. Experimental results showed that GHCA outperformed other models in most transfer cases, with OA ranging from 0.82 to 0.95 (cross-region) and 0.89 to 0.98 (cross-year), achieving an average OA increase of 6.2% and 3.5% in cross-region and cross-year experiments, respectively. These results highlight the strong potential of advanced AI methodologies to deliver robust, quantitative, and transferable solutions for complex geoscientific problems using large Earth observation datasets.

How to cite: Yang, J., Hu, Q., Belgiu, M., and Wu, W.: A global–hierarchical–categorical alignment framework to address sample scarcity and domain shift in crop mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10174, https://doi.org/10.5194/egusphere-egu26-10174, 2026.

This study introduces an innovative methodology for generating realistic soil prediction maps that visualise the spatial distribution of specific chemicals, achieved through the rigorous evaluation and comparison of advanced modelling techniques, including innovative modelling techniques based on the use of neural networks and multilayer perceptrons (MLPs). The Drava River floodplain was selected as the primary case study based on stringent criteria: a) intensive historical metal ore mining and metallurgical processing activities, which have left a legacy of contamination; b) distinctive geomorphological features, such as dynamic floodplains and sediment deposition zones; and c) diverse geological settings that facilitate reliable model calibration across transboundary reaches. Soil measurements were integrated with diverse geospatial datasets—derived from Digital Elevation Models (DEMs), land cover classifications, and remote sensing imagery—to enable high-resolution mapping of contaminant distributions via sophisticated predictive modelling powered by neural networks and MLPs. A novel, holistic approach was applied to simultaneously reconstruct multiple influencing processes, including erosion, sediment transport, and pollutant dispersion, across the entire study area. This comprehensive framework not only advances contamination mapping practices but also empowers the developed models to trace primary distribution pathways, quantify the true extent of affected zones, enhance data interpretability, and inform evidence-based decisions on land-use planning, remediation strategies, and environmental management in mining-impacted regions.

How to cite: Alijagić, J. and Šajn, R.: Advanced AI Soil Mapping Techniques and Transboundary Risk Assessment for the Drava River Floodplain , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10465, https://doi.org/10.5194/egusphere-egu26-10465, 2026.

EGU26-11012 | Posters on site | GI2.1

Deep-learning based large-scale automated observation of earthquake surface ruptures 

Xin Liu, Shirou Wang, Xuhua Shi, Cheng Su, Yann Klinger, Arthur Delorme, Haibing Li, Jiawei Pan, and Hanlin Chen

Rapid and objective mapping of co-seismic surface ruptures is essential for post-earthquake impact assessment and for improving our understanding of fault geometry, stress transfer, and rupture processes that inform longer-term seismic hazard analyses. However, rupture mapping has traditionally relied on manual interpretation of field observations or remote-sensing data, which is time-consuming and difficult to extend consistently to large spatial extents, multiple earthquakes, and diverse data sources. Here we present an automated deep-learning framework—the Deep Rupture Mapping Network (DRMNet)—a convolutional neural network designed for end-to-end, high-precision detection of co-seismic surface ruptures from multi-sensor imagery. DRMNet is applied to four large continental earthquakes: the 2021 Mw 7.4 Maduo, 2022 Mw 6.9 Menyuan, 2001 Mw 7.8 Kokoxili, and 1905 Mw ~8 Bulnay (Mongolia) events. The framework consistently delineates both primary and subsidiary rupture structures across centimetre-scale drone imagery and metre-scale satellite data. Across diverse tectonic settings, image resolutions, and preservation states, DRMNet achieves precisions approaching or exceeding 90%. By enabling consistent rupture recognition across multiple events, sensors, and timescales, the proposed framework overcomes the event-specific and local-scale limitations of previous approaches, supporting both rapid post-earthquake response and retrospective rupture reconstruction, and laying the groundwork for standardized global surface-rupture inventories.

How to cite: Liu, X., Wang, S., Shi, X., Su, C., Klinger, Y., Delorme, A., Li, H., Pan, J., and Chen, H.: Deep-learning based large-scale automated observation of earthquake surface ruptures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11012, https://doi.org/10.5194/egusphere-egu26-11012, 2026.

EGU26-12550 | ECS | Posters on site | GI2.1

Identifying zircon provenances using domain-adversarial neural network 

Mengwei Zhang, Guoxiong Chen, Timothy Kusky, Mark Harrison, Qiuming Cheng, and Lu Wang
  • Zircon trace element geochemistry is a pivotal tool for unraveling petrogenesis and the evolutionary history of the Earth’s crust. While two-dimensional (2D) discriminant diagrams are conventionally used to identify parent rock types, the emergence of machine learning (ML) has introduced a transformative research paradigm. ML not only enhances classification accuracy but also resolves the inherent ambiguities found in traditional geochemical diagrams. However, the reliability of current ML models typically depends on the vast archives of labeled samples from the Phanerozoic. When extending research to “deep-time” samples, such as Hadean zircons, the scarcity of labeled data often forces researchers to rely on models trained exclusively on Phanerozoic datasets. This approach is prone to misclassification due to “domain shift,” caused by systematic variations in zircon trace element distributions across different geological eons. To address this challenge, we propose a Domain Adversarial Neural Network (DANN) framework tailored for zircon trace element analysis. By aligning the feature distributions of the source domain (Phanerozoic) and the target domain (Precambrian), the DANN extracts “domain-invariant yet geologically significant” high-dimensional feature representations, effectively mitigating the effects of temporal data bias. Our results demonstrate that DANN significantly outperforms traditional machine learning methods across multiple performance metrics. Furthermore, t-SNE visualization confirms that the source and target domains are effectively aligned within the feature space. When applied to ~4.3 Ga zircon samples from the Jack Hills, the model achieved a classification accuracy of 0.923. This high level of performance underscores the framework’s exceptional generalization capability for identifying unlabeled deep-time samples and its potential for broader applications in Precambrian geology. This study develops a transferable, data‑driven framework for inferring deep‑time geological processes, providing a novel methodology to address the limitations inherent in the traditional principle of uniformitarianism. Furthermore, the framework is extensible to other mineral systems (e.g., apatite, monazite), thereby opening new avenues for quantitatively reconstructing the dynamic evolution of the early Earth.

How to cite: Zhang, M., Chen, G., Kusky, T., Harrison, M., Cheng, Q., and Wang, L.: Identifying zircon provenances using domain-adversarial neural network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12550, https://doi.org/10.5194/egusphere-egu26-12550, 2026.

EGU26-13366 | ECS | Orals | GI2.1

Spatial Downscaling of Land Surface Temperature Using Sentinel-2 and Sentinel-3 Data Fusion for Agricultural Applications 

Bouchra Boufous, Fatima Ben zhair, and Salwa Belaqziz

Land surface temperature (LST) is a key variable for assessing crop thermal stress and supporting precision agriculture. However, thermal satellite products often involve a trade-off between spatial and temporal resolution. Sentinel-3 provides frequent LST observations, but its coarse spatial resolution limits its use for field-scale agricultural monitoring.

This study proposes a spatial downscaling approach for LST based on the fusion of Sentinel-3 thermal data with high-resolution multispectral information from Sentinel-2. The method exploits the inverse relationship between surface temperature and vegetation cover through the Normalized Difference Vegetation Index (NDVI). A linear regression model was developed to estimate LST at a spatial resolution of 10 m using Sentinel-2 NDVI as the primary predictor.

The approach was applied over the agricultural site of El Ghaba in the Marrakech–Safi region (Morocco), covering different crop types, including annual cereals (barley, wheat, and kerenza) and perennial olive orchards. Results show a clear negative correlation between NDVI and LST, confirming the regulatory role of vegetation on surface temperature. The downscaled LST maps reveal fine-scale spatial heterogeneity that is not detectable in the original Sentinel-3 product.

Quantitative evaluation indicates low absolute errors for annual crops (generally below 0.5 °C), demonstrating the robustness of the proposed method, while higher discrepancies observed for olive orchards highlight the complexity of perennial crop thermal behavior. This work enhances the spatial usability of satellite thermal data for agricultural monitoring and crop stress assessment.

How to cite: Boufous, B., Ben zhair, F., and Belaqziz, S.: Spatial Downscaling of Land Surface Temperature Using Sentinel-2 and Sentinel-3 Data Fusion for Agricultural Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13366, https://doi.org/10.5194/egusphere-egu26-13366, 2026.

EGU26-13941 | Orals | GI2.1

Why Automated Mineralogy needed an upgrade 

Rich Taylor

Automated Mineralogy – the past

The automated classification of mineral phases in rocks has been a mainstay of the Geoscience analytical community for over 40 years. While we have seen great leaps forward in AI in µCT and light microscopy/petrography, the automated capabilities for the SEM have progressed and changed very little in decades, relying heavily on outdated methods that were available at the time.

The technology come with several significant problems moving forward, including excessive hardware-software dependencies, complex mineral libraries and classifications, inconsistent user experience, and difficult workflows outside their intended use.

 

Recent technological advances

There are two broad shifts that are taking place across a number of microscopy and microanalysis techniques – the acquisition of more quantitative data, and the application of deep learning neural networks. As a general trend this can be thought of as building better datasets, and building bigger datasets.

EDS as a SEM-based technique is fertile territory for both of these shifts. As an analytical technique EDS is commonly applied qualitatively, or as an image based method for distinguishing regions based on chemical maps. In recent years it has become easier than ever before to calibrate systems and detectors for concentration data, meaning the SEM can generate more robust datasets without having to fall back on other techniques.

Deep Learning is a topic that covers a broad range of mathematical applications to everything from the acquisition of microscopy datasets, through to data processing and interpretation across almost all sciences. There are many different flavours of deep learning neural network (DLNN) and each type lends itself to different applications, particularly in the varied data rich environments of microscopy. DLNN are inherently hard to track exactly how they operate, but at their best should be easy to use, and easy to understand how they’ve been applied to a scientific problem.

 

Automated Mineralogy – the future

The introduction of both quantitative mineral chemistry and DLNN to automated mineral classification is a huge leap forward, solving many of the problems of traditional software. Detaching data acquisition from processing removes software dependencies and frees users to build their ideal system. An DLNN-driven, unsupervised data processing approach can be data led rather than user led, making it more robust and consistent across instruments and facilities. Quantitative analysis can build on the DLNN approach by allowing a “best fit” classification, removing the need for constant modification of mineral libraries, and simply allowing “textbook” globally consistent mineral compositions to drive the labelling of segmented data.

How to cite: Taylor, R.: Why Automated Mineralogy needed an upgrade, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13941, https://doi.org/10.5194/egusphere-egu26-13941, 2026.

EGU26-14415 | ECS | Orals | GI2.1

Multi-agent Geochemical Literature Data Mining System 

Tianyu Yang, Karim Elezabawy, Daniel Kurzawe, Leander Kallas, Marie Traun, Bärbel Sarbas, Adrian Sturm, Stefan Möller-McNett, Matthias Willbold, and Gerhard Wörner

The increasing volume and complexity of geochemical literature pose major challenges for the sustainable curation of domain-specific databases such as GEOROC (Geochemistry of Rocks of the Oceans and Continents), the world’s largest repository of geochemical and isotopic data from igneous and metamorphic rocks and minerals, aggregating more than 41 million values from over 23,000 publications. Although GEOROC underpins a wide range of geoscientific research, the extraction and harmonization of metadata from publications still relies heavily on manual effort, which significantly limits the scalability.

In this contribution, we present a novel information extraction architecture that moves beyond linear processing pipelines toward an Large Language Model (LLM)-based multi-agent system combining document layout analysis, schema-driven reasoning, and modality-aware extraction. Unlike generic LLM approaches that treat documents as continuous text streams, our architecture adopts a "Visual-First" strategy. We utilize a layout-aware backbone (MinerU, Niu et al., 2025) to decompose PDF manuscripts into a sequence of geometrically grounded primitive blocks, each representing a localized document region with associated visual and typographic features, preserving the geometric grounding essential for interpreting complex data tables. A routing agent subsequently validates and refines the initial layout classification, dynamically dispatching blocks to specialized downstream agents for text, table, or figure processing. This adaptive routing strategy improves robustness against layout variability across journals, publication years, and formatting styles.

Central to the framework is an active schema agent that operationalizes the GEOROC metadata model. Rather than treating the database schema as a static template, this agent continuously provides extraction targets, normalization rules, unit standards, and conflict-resolution policies that guide all subsequent processing steps. Text blocks are handled by an  Optical Character Recognition (OCR) driven information extraction agent, table blocks by a table parsing agent capable of reconstructing complex table structures, and figure blocks by a visual reasoning agent designed to interpret diagrams and digitize plotted values. Each agent produces structured candidate values enriched with confidence estimates and fine-grained provenance, including page-level and bounding-box references to the original document.

The outputs of these modality-specific agents are consolidated by a merge-and-judge agent, which goes beyond simple aggregation. This agent performs cross-modal arbitration, unit harmonization, and deduplication, resolving conflicts between heterogeneous sources according to schema-defined priorities and data-quality criteria. The final result is a machine-readable JSON representation that preserves both extracted values and their evidential context.

By combining layout grounding, adaptive routing, schema-driven reasoning, and judgment-based integration, this system delivers a robust and extensible approach to large-scale metadata extraction. The framework substantially supports the curation process and strengthens GEOROC’s role as a FAIR-compliant reference infrastructure by enabling more efficient reuse of published geochemical data in future geochemical research.

References:

Niu, J., Liu, Z., Gu, Z., Wang, B., Ouyang, L., Zhao, Z., ... & He, C. (2025). Mineru2. 5: A decoupled vision-language model for efficient high-resolution document parsing. arXiv preprint arXiv:2509.22186.

How to cite: Yang, T., Elezabawy, K., Kurzawe, D., Kallas, L., Traun, M., Sarbas, B., Sturm, A., Möller-McNett, S., Willbold, M., and Wörner, G.: Multi-agent Geochemical Literature Data Mining System, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14415, https://doi.org/10.5194/egusphere-egu26-14415, 2026.

EGU26-14874 | ECS | Posters on site | GI2.1

Quartz grain microtexture analysis using Artificial Intelligence: application to tsunami and storm deposits provenance studies 

Natércia Marques, Pedro Costa, and Pedro Pina

Quartz grain surface microtextures observed by scanning electron microscopy (SEM) provide important information on sediment transport history, depositional processes and sediment provenance. Traditionally, the interpretation of these features has relied upon qualitative visual assessment—an approach deeply rooted in expert judgement and cumulative experience. While fundamental, this methodology is inherently susceptible to subjectivity and inter-analyst variability. To counter balance this problem, we explore image-based classification approaches (utilizing Deep Learning frameworks) as a tool to support quartz microtextural analysis and assist in the identification of likely depositional environments thus establishing sediment provenance relationships.

A dataset of 3 367 SEM images was compiled, spanning a diverse range of sedimentary contexts: aeolian dunes, beach faces’, alluvial systems, basal sands, and nearshore, alongside with high-energy deposits from storm and tsunami events. Based on this dataset, five classification models were developed. Three were designed to discriminate between the full set of seven depositional classes, while two focused on a reduced classification scheme comprising four classes (alluvial, beach, dune and nearshore). All models were optimised using an increasing number of training epochs to assess the stability and evolution of classification performance. The results obtained were further examined in comparison with SandAI, an existing tool for microtexture classification, to evaluate its behaviour when applied to new sedimentary contexts and datasets acquired under different conditions.

The most consistent classification results were obtained for environments characterised by well-preserved and distinctive mechanical microtextures (e.g. aeolian sediments). Conversely, while environments defined by overlapping processes occasionally yielded higher nominal accuracies in QzTexNet (CNN-based models developed within the scope of this work), this is potentially attributed to their over-representation in the dataset. Analysis of classification outcomes indicates that microtextural overprinting, dataset imbalance and variations in image quality reduced the visibility of diagnostic features, thereby complicating the differentiation of depositional settings. Nevertheless, the data suggests that our models successfully capture sedimentologically meaningful patterns when surface textures remain clear. While SandAI showed stable performance within its original scope, its accuracy was limited, peaking at 47% for its target environments and dropping significantly when faced with complex deposits like tsunami or nearshore grains. In contrast, the newly developed QzTexNet models showed slightly more encouraging results, reaching accuracies of around 55% and demonstrating a steady improvement through successive refinements.

Ultimately, these findings demonstrate that automated classification offers a powerful complement to traditional analysis, particularly in ensuring reproducibility across large-scale datasets. Solely based on our database, it was observed that challenges regarding dataset equilibrium and textural complexity persist, targeted methodological refinements and supervised training hold significant potential. Such advancements represent a promising frontier in sedimentary provenance studies, particularly for the rigorous identification of deposits linked to extreme geological events.

This work is supported by FCT, I.P./MCTES through national funds (PIDDAC): LA/P/0068/2020 (https://doi.org/10.54499/LA/P/0068/2020), UID/50019/2025(https://doi.org /10.54499/UID/PRR/50019/2025), UID/PRR2/50019/2025). Finally this work is a contribution to project iCoast (project 14796 COMPETE2030-FEDER-00930000).

How to cite: Marques, N., Costa, P., and Pina, P.: Quartz grain microtexture analysis using Artificial Intelligence: application to tsunami and storm deposits provenance studies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14874, https://doi.org/10.5194/egusphere-egu26-14874, 2026.

Wildfires are increasingly reshaping landscapes across the U.S., disrupting hydrogeologic processes such as runoff, infiltration, and sediment transport—posing major challenges for streamflow prediction and water resource management. Traditional conceptual and physically based hydrologic models often struggle to capture these disturbance-driven dynamics. In this study, we explore the potential of long short-term memory (LSTM) networks, a type of recurrent neural network, to simulate post-fire streamflow across 1,082 fire-affected basins spanning the contiguous U.S.—representing the first near-continental-scale application of LSTMs for wildfire-related hydrologic prediction. 

Three LSTM models were trained on different temporal splits of fifteen-year datasets containing wildfire events: one using pre-fire data, one using post-fire data, and one using the full dataset. Models were evaluated on unseen basins in both pre- and post-fire windows. Results show that the model trained on the full dataset consistently outperformed the others, underscoring the importance of temporally diverse training data that include disturbance events. Importantly, LSTMs demonstrated strong generalization across disturbed and undisturbed environments, highlighting their ability to learn hydrologic patterns beyond the constraints of traditional process-based modeling frameworks. 

Feature importance analysis revealed that topographic variables (e.g., elevation and slope) were most influential, followed by soil/geologic and vegetation characteristics, while fire-specific indicators (e.g., burn severity) ranked surprisingly low. This suggests that the LSTMs internalized key controls on streamflow response without heavy reliance on the explicit disturbance metrics included. To further isolate the model’s learned response to wildfire, simulations were performed with synthetic unburned conditions for each disturbed basin and compared against burned scenarios. Spatial analysis by EPA Level II ecoregion revealed that in the Southeastern U.S., Ozark/Appalachian Forests, and Mediterranean California, the model identified a persistent, multi-year increase in streamflow-lasting up to three years after wildfire. These regions share ecological characteristics such as high vegetation biomass, seasonal climate regimes, and terrain-driven hydrologic gradients that collectively amplify post-fire reductions in evapotranspiration and enhance runoff generation. In contrast, no significant streamflow change was detected in the Western Cordillera, South Central Prairies or Cold Desert ecoregions, where water-limited climates and lower fuel loads results in a dual-action response of hydrologic buffering and constrained post-fire increases in water yield.    

Together, these findings demonstrate that LSTMs can detect regionally coherent hydrologic responses to wildfire even in the absence of strong dependence on explicit disturbance features, highlighting the promise of AI-driven, data-centric approaches for modeling hydrologic change in an era of increasing disturbances. As wildfires and other extreme events become more frequent, integrating machine learning into hydrologic prediction frameworks offers a powerful pathway toward adaptive water resource management and improved resilience across diverse ecohydrologic settings. 

How to cite: Hogue, T., Moon, C., and Corona, C.: Quantifying Post‑Wildfire Hydrologic Response Using LSTMs: Ecoregion Patterns Across the Contiguous United States, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15295, https://doi.org/10.5194/egusphere-egu26-15295, 2026.

EGU26-15913 | ECS | Posters on site | GI2.1

AI-assisted Remote Sensing Screening of Potential Natural Hydrogen Seepage Features in Alta Guajira, Northern Colombia 

Miguel Angel Monterroza Montes, Stephanie San Martín Cañas, Boris Lora-Ariza, and Leonardo David Donado

Natural (geological) hydrogen refers to molecular hydrogen produced in the subsurface through abiotic and biogenic pathways, which may migrate, accumulate transiently, be consumed by secondary reactions, or escape to the surface. Increasing evidence indicates that such systems could be a strategic low-carbon energy source, but their exploration is limited as regional-scale, data-driven approaches to identify mechanisms of active or fossil migration in geologically complex environments are lacking. Surface expressions such as circular and sub-circular depressions associated with soil and vegetation anomalies have been reported worldwide as indirect indicators of hydrogen migration and leakage. However, their detection remains limited to either local reconnaissance of the field or manual interpretation of remote-sensing data. In this research, we present an AI-assisted remote sensing framework to conduct a regional screening based on the potential for natural hydrogen seepage patterns to enhance early-stage exploration and improve the quantitative characterization of surface indicators linked to subsurface energy systems. Deep-learning–based computer vision models are used to study high-resolution satellite imagery and automatically identify and classify circular and sub-circular geomorphological features that could correspond to hydrogen exudation. The resulting detections are integrated into a GIS framework for the extraction of morphometric and spatial statistics, providing a formal analytical benchmark to relate surface structures to lithology, structural configuration, and the regional tectonic setting. The workflow is applied to the Alta Guajira region (in northern Colombia), a geologically complex segment of the Caribbean margin characterized by accreted oceanic crust, major fault systems, and sedimentary depocenters that may favor hydrogen generation and migration. Using an AI-based approach allows the construction of a regional inventory of candidate seepage-related structures while significantly reducing false positives associated with purely morphology-based analyses. The results support the prioritization of targets for future field verification, geochemical sampling, and subsurface investigations. Beyond its implications for natural hydrogen prospectivity, the proposed methodology demonstrates how artificial intelligence can translate qualitative geological observations into quantitative, reproducible screening tools. By providing a transparent and spatially explicit representation of subsurface energy systems, AI-assisted screening also facilitates communication with stakeholders and local communities, contributing to informed public perception of emerging sustainable subsurface energy resources in data-limited regions such as Alta Guajira.

The researchers thank the SHATKI Research Project (code 110563), Contingent Recovery Contract No. 112721-042-2025, funded by the Ministry of Science, Technology and Innovation (Minciencias) and the National Hydrocarbons Agency (ANH).

How to cite: Monterroza Montes, M. A., San Martín Cañas, S., Lora-Ariza, B., and Donado, L. D.: AI-assisted Remote Sensing Screening of Potential Natural Hydrogen Seepage Features in Alta Guajira, Northern Colombia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15913, https://doi.org/10.5194/egusphere-egu26-15913, 2026.

EGU26-16953 | ECS | Orals | GI2.1

Local Similarity-Driven Refinement for Model-Agnostic Ground-Based Cloud Detection 

Yangfan Hu, Pinglv Yang, Zeming Zhou, Ran Bo, Shuyuan Yang, and Guangyang Zhang

Cloud cover estimation is of crucial significance in meteorological observations and short-term/long-term weather forecasting, as it directly affects the accuracy of radiation balance assessment, precipitation prediction, and climate change modeling. Ground-based automated cloud quantification observation instruments enable continuous, high-resolution cloud monitoring with spatial-temporal continuity that satellite remote sensing cannot fully achieve, highlighting the immense value of ground-based cloud image processing for practical meteorological applications. However, existing cloud detection methods predominantly rely on supervised training with ground truth masks, which overlook the rich contextual information and inherent regularization constraints embedded in original cloud images. This oversight frequently results in mismatched cloud boundaries, inadequate model interpretability, and poor adaptability to complex cloud morphologies—particularly for thin clouds and cirrus clouds characterized by weak grayscale contrast, sparse texture, and irregular shapes. Consequently, these limitations lead to suboptimal detection performance, including under-segmentation or over-segmentation, and further induce inaccuracies in quantitative cloud cover estimation.

To address the aforementioned issues and achieve accurate cloud cover detection results, this study proposes a model-agnostic refinement method designed to optimize the coarse detection masks generated by any pre-trained cloud detection model. The framework is jointly optimized by three loss functions: a local similarity descriptor, total variation (TV) regularization, and a traditional detection loss (e.g., cross-entropy). Specifically, the local similarity descriptor is defined as the difference between two terms: the average grayscale difference of each pixel and cloud region and background pixels within a local window. This descriptor effectively enhances the discriminability between cloud and non-cloud regions at the local level. The total variation regularization term is introduced to maintain the smoothness of the detection boundary and suppress spurious noise. The cross-entropy loss ensures the overall consistency between the refined result and the ground truth.

Minimizing the combined loss function drives the coarse detection result to evolve adaptively along the actual cloud boundary, thereby achieving more precise alignment with the true cloud contours. Notably, the proposed framework elevates the detection of thin clouds and cirrus clouds, effectively mitigating missed detection areas in these tenuous cloud structures. Furthermore, the integrated loss function enhances model interpretability: the local similarity descriptor explicitly quantifies the differences within local window, and minimizing this term inherently refines the detection by strengthening the distinction between cloud and background regions. Ultimately, the refined detection results substantially improve the accuracy of cloud cover estimation, laying a solid foundation for reliable meteorological observations and weather forecasting applications.

How to cite: Hu, Y., Yang, P., Zhou, Z., Bo, R., Yang, S., and Zhang, G.: Local Similarity-Driven Refinement for Model-Agnostic Ground-Based Cloud Detection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16953, https://doi.org/10.5194/egusphere-egu26-16953, 2026.

Earth Observation (EO) is an essential source of information for most geosciences. However, high costs, large data volumes, and difficult access constrained its use for decades. Open data programs like Copernicus have reduced costs, and cloud access via the Copernicus Data Space Ecosystem (CDSE) has made local processing largely obsolete. In fact, API (Application Programming Interface)-based cloud access, analysis-ready mosaics and calibrated Copernicus Land Monitoring Service data products have made Sentinel data AI-ready. But despite these advances, the requirement for complex programming skills remained a significant barrier until recently. Here, we demonstrate how cloud-native processing APIs and generative artificial intelligence (AI) are removing this obstacle by enabling the "vibe coding" paradigm shift. Vibe coding is an approach to software development where the researcher focuses on the high-level logic, the functional vision, and the end product, while the syntax and code are generated and refined by AI.
Copernicus Data Space Ecosystem facilitates this transition through three key features: (1) the abstraction of EO analysis pipelines via RESTful APIs, which reduces tasks to a series of mathematical operations on pixel values; (2) the availability of intuitive web browser visualization for rapid prototyping and debugging; and (3) an extensive body of open documentation and code examples that serve as a robust training foundation for generative AI.
On CDSE, the Sentinel Hub API family utilizes "custom scripts" (or "evalscripts") — modular JavaScript files defining data inputs, outputs, calculations, and visualizations. The openEO API uses "process graphs", JSON representations of the processing steps in a unified structure as a series of nodes. Because the backend manages big data optimization and the browser handles rendering, these scripts are concise enough for AI assistants to generate, adapt, and debug effectively. The Sentinel Hub Custom Script Repository, containing over 200 community-contributed scripts, and the openEO community examples repository and CDSE "Algorithm Plaza" have laid the foundation for this approach. Neither of these advances was intentionally created to support AI, but rather to simplify programming for humans; however, combined, they enable a breakthrough in code development. We demonstrate how AI tools can efficiently adapt scripts across different satellite sensors, combine spectral indices into decision trees, and produce scalable quantitative outputs. This allows researchers not specialized in remote sensing to utilize existing code modules and natural language prompts to create meaningful results for their specific fields. Beyond the capabilities of Sentinel Hub, OpenEO supports joint analysis of data from multiple back-ends and the application of user-defined external code, such as biophysical models or pre-trained ONNX deep learning networks. While this added complexity presents a higher technical threshold, it also creates a massive opportunity for AI-driven automation. Ultimately, in combination with the public data space approach, generative AI further democratizes Earth Observation, transforming it from a specialist-only domain into an integrated component of all geoscience research workflows.

How to cite: Zlinszky, A.: From natural language to quantitative satellite imagery analysis: Copernicus Data Space Ecosystem and AI enable vibe coding of custom scripts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18394, https://doi.org/10.5194/egusphere-egu26-18394, 2026.

EGU26-18939 | ECS | Posters on site | GI2.1

Evaluating Fractional Vegetation Cover using Multimodal Large Language Models: A Comparative study with Human Observations 

Omar A. Lopez Camargo, Mariana Elias Lara, Marcel El Hajj, Hua Cheng, Dario Scilla, Victor Angulo, Areej Al wahas, Kasper Johansen, and Matthew F. McCabe

Fractional Vegetation Cover (FVC) is a key ecological variable for monitoring ecosystem health, land degradation, and vegetation dynamics in dryland environments. While satellite and UAV observations enable scalable FVC estimation over large spatial extents, the accuracy and robustness of these models remain strongly dependent on high-quality field-based reference data for calibration and validation. Traditional in-situ methods, including visual estimates using transect-based surveys, remain widely used but are labor-intensive and inherently subjective. Digital photography has emerged as a practical alternative, typically analyzed using index-based computer vision techniques or deep learning models. However, these methods are highly sensitive to background variability and therefore rely on massive labeled datasets. Recent advances in multimodal large language models (MLLMs) suggest a potential paradigm shift, as these models combine visual perception with high-level reasoning and benefit from diverse pre-training that enables conceptual knowledge transfer across tasks. In this study, we evaluate the feasibility of using MLLMs for direct estimation of FVC from ground-level photographs without task-specific training. We collected and compiled a dataset of more than 1,100 quadrat pictures from across 26 dryland sites in Saudi Arabia, spanning a wide range of surface conditions from bare soil to sparsely vegetated rangelands. Each picture corresponded to a 1 m × 1 m quadrat with FVC estimated independently by two experts, whose average was used as reference data for assessment of model predictions. Six state-of-the-art multimodal large language models, including Qwen2.5-VL, Mistral-Small-3.2, LLaMA-4-Maverick, LLaMA-4-Scout, and two Gemma-3 variants, were evaluated using four prompt designs that varied in length, ecological context, and methodological detail. Across all models and prompts, MLLMs achieved a mean absolute error of approximately 7.8%, demonstrating competitive performance relative to traditional image-based methods. The best-performing model-prompt combinations achieved mean absolute error values below 5%, with low systematic bias. Short and ecologically explicit prompts consistently outperformed more complex prompt designs, achieving an average reduction in mean absolute error (MAE) of approximately 1.3–1.4 percentage points compared to visually guided or highly structured prompts (MAE ≈ 6.9% versus 8.2–8.4%). Overall performance was more sensitive to model choice than to prompt structure, with mean MAE varying from approximately 5.6% to 10.0% across models, compared to a narrower range across prompts. The highest accuracy was obtained using the Qwen2.5-VL model with an ecologically detailed prompt, which achieved a mean absolute error of 4.9%, near-zero bias, and an RMSE of 8.4%. Across all prompt designs, Qwen2.5-VL and Mistral-Small-3.2 consistently delivered the best overall performance, both maintaining mean MAE values below 6% and exhibiting stable behavior across prompt variations, indicating robustness to prompt design. These results demonstrate that MLLMs can provide accurate and scalable FVC estimates directly from field photographs, without requiring specialized training datasets. This approach offers a promising alternative for rapid field surveys and reference data generation, particularly in dryland ecosystems where background complexity and data scarcity limit the effectiveness of conventional methods.

How to cite: Lopez Camargo, O. A., Elias Lara, M., El Hajj, M., Cheng, H., Scilla, D., Angulo, V., Al wahas, A., Johansen, K., and McCabe, M. F.: Evaluating Fractional Vegetation Cover using Multimodal Large Language Models: A Comparative study with Human Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18939, https://doi.org/10.5194/egusphere-egu26-18939, 2026.

Earth system is characterized by intricate interactions between human activities and natural processes, where stochastic dynamics, nonlinear feedbacks, and emergent behaviors collectively determine system evolution and sustainability outcomes. Despite significant advances in Earth system science, two fundamental challenges persist: the insufficient integration of physical process models with observational data, and the lack of interpretable frameworks for simulating coupled human-Earth dynamics and optimizing governance strategies. These limitations critically impede our ability to conduct effective Earth system governance and guide human-environment interactions toward sustainable development pathways. To overcome these challenges, this study proposes an innovative framework that synergistically integrates data assimilation and reinforcement learning to enhance both predictability and decision-making capabilities in the complex Earth system. Data assimilation, as a well-established methodology in Earth system science, systematically combines dynamic models with multi-source observations to improve system observability and forecast accuracy. Reinforcement learning, grounded in the Bellman equation and Markov decision processes, provides a natural paradigm for modeling adaptive human-environment interactions and deriving optimal strategies through sequential decision-making under uncertainty. Building upon these complementary methodologies, we develop a Multi-Agent Deep Reinforcement Learning (MADRL) framework that employs the Markov decision process as the theoretical foundation, integrates agent-based modeling to represent heterogeneous stakeholder behaviors across multiple organizational levels, utilizes deep neural networks to handle high-dimensional state-action spaces, and incorporates data assimilation techniques to continuously update system states and reduce forecast uncertainties. This integrated framework is specifically designed to address fundamental Earth system governance challenges by capturing emergent phenomena arising from complex human-environment interactions, enabling the exploration of intervention mechanisms such as economic incentives, regulatory policies, and cooperative arrangements, and providing interpretable decision pathways that balance economic development with environmental sustainability. Through this integration, our framework offers a systematic approach to tackle classical problems in Earth system governance, from the tragedy of the commons to planetary boundaries, ultimately advancing our capacity to navigate toward sustainable development trajectories in an increasingly coupled human-Earth system.

How to cite: Yuan, S. and Li, X.: Generalizing human-Earth systems modeling and decision-making: A multi-agent deep reinforcement learning framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19409, https://doi.org/10.5194/egusphere-egu26-19409, 2026.

EGU26-19427 | Posters on site | GI2.1

Improving the seismic catalogue completeness of Tenerife (Canary Islands, Spain) through deep learning 

Manuel Calderón-Delgado, Luca D’Auria, Aarón Álvarez-Hernández, Rubén García-Hernández, Víctor Ortega-Ramos, David M. van Dorth, Sergio de Armas-Rillo, Pablo López-Díaz, and Nemesio M. Pérez

The volcanic island of Tenerife (Canary Islands, Spain) is characterized by low-magnitude background seismicity associated with local hydrothermal and volcano-tectonic processes. The island has been experiencing, since 2016, a slight increase in seismic activity, with earthquakes generally having magnitudes below 2. For this reason, we are revising the seismic catalogue using deep learning tools to improve its completeness.

Over the last decade, machine learning methods—particularly deep learning approaches—have gained traction across multiple disciplines due to their increased computational efficiency, high accuracy, and reduced need for manual supervision. One such method, PhaseNet [1], is a deep convolutional neural network based on the U-Net architecture [2] that has shown strong performance in waveform-based seismic phase detection. Its ability to process large volumes of seismic data and automatically identify relevant signal features represents a significant opportunity to enhance the quality and completeness of seismic catalogs. Nevertheless, applying a neural network to data with a different nature from that used for its training phase can lead to a substantial decrease in performance. In particular, PhaseNet was primarily trained on tectonic seismicity, whereas seismic events in Tenerife are predominantly volcanic-hydrothermal. Consequently, retraining the network on waveforms representative of the target seismicity is essential to ensure a reliable inference.

Using PhaseNet as a baseline, we conducted an extensive comparative analysis of several training configurations to adapt the original network to the seismic data from the Canary Islands (Tenerife). Our study focused on four key aspects: model initialization, learning rate selection, data clustering strategies, and model partitioning. The model initialization strategies include fine-tuning from pre-trained weights and training from randomly initialized weights. Regarding model partitioning, we evaluated a global model (a single model trained on all data), local models (one model per station), and cluster-based models (trained on groups of stations with similar characteristics). The performance of each configuration was evaluated on an independent dataset using multiple metrics to provide a comprehensive assessment. Specifically, we analyzed precision, recall, and ROC curves to identify suitable trade-offs between detection sensitivity and specificity.

These preliminary results will be beneficial for subsequent analysis aimed at a better characterization of the island's microseismicity and its relationship with the activity of its volcanic-hydrothermal system.

References:

  • [1] Zhu and G. C. Beroza, “PhaseNet: a Deep-Neural-Network-Based seismic arrival time picking method,” Geophysical Journal International, Oct. 2018, doi: 10.1093/gji/ggy423.
  • [2] O. Ronneberger, P. Fischer, and T. Brox, “U-NET: Convolutional Networks for Biomedical Image Segmentation,” in Lecture notes in computer science, 2015, pp. 234–241. doi: 10.1007/978-3-319-24574-4_28.

 

How to cite: Calderón-Delgado, M., D’Auria, L., Álvarez-Hernández, A., García-Hernández, R., Ortega-Ramos, V., M. van Dorth, D., de Armas-Rillo, S., López-Díaz, P., and M. Pérez, N.: Improving the seismic catalogue completeness of Tenerife (Canary Islands, Spain) through deep learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19427, https://doi.org/10.5194/egusphere-egu26-19427, 2026.

EGU26-19439 | ECS | Posters on site | GI2.1

Onboard Hybrid Orbit Prediction with Lightweight Machine-Learning Error Correction 

Benedikt Aigner, Fabian Dallinger, Thomas Andert, and Benjamin Haser

Autonomous spacecraft operations are increasingly important as missions grow more complex, ground contact opportunities remain limited, and the number of LEO satellites continue to rise. Reliable onboard orbit determination (OD) and orbit prediction (OP) are essential for mission planning, resource allocation, and communication scheduling. Operational OD/OP typically relies on physics-based models that estimate parameters (initial state, drag coefficient, etc.) from tracking data. However, environmental modeling is not perfect, and uncertainties in atmospheric density can cause prediction errors to grow rapidly. This limits OP reliability.

We present an onboard-oriented hybrid OD/OP concept that augments a classical physics-based OD/OP chain with a lightweight machine-learning (ML) correction module to compensate for systematic OP errors in real time. While data-driven correction of propagator errors has been explored previously, this work emphasizes the tight integration of a compact correction model into an operational workflow under onboard constraints. The implementation is based on the Python OD/OP toolbox Artificial Intelligence for Precise Orbit Determination (AI4POD) and targets deployment within the Autonomous Space Operations Planner and Scheduler (ASOPS) experiment, that is planned for validation on the ATHENE-1 satellite.

The approach is demonstrated using simulated GPS-like tracking data generated with a high-fidelity reference model, while OD/OP are performed with a reduced-complexity model representative of onboard settings. A compact artificial neural network (ANN) is trained to predict OP errors in the RSW frame from available onboard data, reducing the maximum three-day along-track error from ~5 km to ~1.2 km.

To assess operational robustness, we complement the baseline results with a statistical consistency check of the residuals across all prediction cases and outline planned tests with additional ML/DL correction models.

How to cite: Aigner, B., Dallinger, F., Andert, T., and Haser, B.: Onboard Hybrid Orbit Prediction with Lightweight Machine-Learning Error Correction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19439, https://doi.org/10.5194/egusphere-egu26-19439, 2026.

EGU26-19927 | ECS | Posters on site | GI2.1

Single- vs. Multilayer Physics-Informed Extreme Learning Machines for Orbit Determination 

Fabian Dallinger, Benedikt Aigner, Thomas Andert, and Benjamin Haser

Orbit Determination (OD) is commonly addressed with classical estimators such as Weighted Least Squares, which are statistically well founded but can be sensitive to poor initialization and may degrade when the initial state is weakly known. Physics-Informed Machine Learning offers an alternative by embedding orbital dynamics directly into the estimation process. In this work, Physics-Informed Extreme Learning Machines (PIELMs) are investigated as fast OD models that do not require a high-quality initial guess, since the output layer is obtained from a physics-based training objective that enforces consistency with both measurements and dynamics.

While single-layer PIELMs can achieve high accuracy, they may exhibit reduced stability in regimes with limited measurement support. To improve representational capacity and generalization, the Deep PIELM augments the model with an autoencoder-based feature hierarchy that is pretrained efficiently via the Moore–Penrose pseudoinverse, followed by physics-informed nonlinear least-squares optimization of the final layer.

Comparative results highlight the trade-offs among classical least squares, single-layer PIELM, and Deep PIELM in terms of OD accuracy, robustness under poor initialization, and computational efficiency under sparse optical and range measurements from a limited set of ground stations. For suitable hyperparameter configurations, the multilayer architecture provides improved stability and accuracy over the single-layer variant while retaining low training times, positioning Deep PIELMs as an effective complement to classical least-squares OD when robust performance without reliable initial guesses is required. The presented work is part of the Artificial Intelligence for Precise Orbit Determination project.

How to cite: Dallinger, F., Aigner, B., Andert, T., and Haser, B.: Single- vs. Multilayer Physics-Informed Extreme Learning Machines for Orbit Determination, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19927, https://doi.org/10.5194/egusphere-egu26-19927, 2026.

EGU26-20311 | ECS | Orals | GI2.1

Performance Comparison of Some Artificial Intelligence Algorithms for Metallic Mineral Deposits: A Case from Türkiye 

Gizem Karakas, Bahunur Civci, Birgul Topal, Candan Gokceoglu, Ahmet Ozcan, Cagri Erbasli, F. Sumeyye Cebeloglu, Murat Koruyucu, and Banu Ebru Binal

Recent advances in artificial intelligence and geospatial data analytics have led to an increasing adoption of data-driven approaches in the identification and prediction of mineral deposits. Traditional mineral exploration methods often rely on single data sources or expert-driven interpretations and may therefore be inadequate in regions where geological information is limited or spatially complex. In contrast, artificial intelligence–based approaches enable the quantitative assessment of mineral potential and the identification of spatial patterns associated with mineralization by jointly integrating multi-source geological, geophysical, and remote sensing data. Therefore, the comparative evaluation of different artificial intelligence algorithms using approaches that account for spatial dependence is critical for selecting reliable and interpretable models in early-stage mineral exploration conducted under data-limited conditions.

This study focuses on a comparative evaluation of artificial intelligence algorithms for predicting potential iron (Fe) mineralization under limited geological data conditions in a region with metallic mineralization potential in Türkiye. The study area covers approximately 2,340 km². A total of seven predictor variables were incorporated into the modeling, classified into geological (lithology, geological age, formation type), structural (fault density), geophysical (magnetic anomaly and gravity-tilt features), and remote sensing–based datasets (iron oxide potantial zones derived from ASTER imagery). The mineralization inventory is highly sparse, comprising only 15 iron occurrences and 24 non-iron reference points selected by geologists To address this limitation, a spatially aware hard negative mining strategy was applied, in which negative samples were preferentially selected from areas spatially proximal to known mineralization occurrences. Model performance was evaluated using GroupKFold-based spatial cross-validation to minimize bias arising from spatial autocorrelation, within which the Random Forest (RF) and XGBoost (XGB) algorithms were compared. The obtained results show that the RF and XGB models achieved mean Area Under Curve (AUC) values of 0.85 and 0.89, respectively. According to the generated mineral prospectivity maps, the Random Forest model delineates approximately 207.02 km² of high-potential areas (probability ≥ 0.90), while the XGBoost model identifies high-potential areas covering approximately 404.04 km² at the same probability threshold. These results indicate that there are pronounced differences in the spatial distribution of high-potential areas depending on the algorithm used. Additionally, the feature importance analysis revealed that geological age, magnetic anomaly, formation type, and gravity-tilt features are the primary controlling factors influencing the spatial distribution of iron mineralization.

This study outcomes revealed the importance of algorithm selection and spatially aware validation strategies in artificial intelligence–based mineral exploration. The findings indicate that reliable mineral prospectivity assessments can be achieved even under limited geological data conditions. Furthermore, in early-stage exploration programs, these approaches strengthen effective target area prioritization and decision-support processes and contribute to cost reduction through more efficient planning of exploration activities.

How to cite: Karakas, G., Civci, B., Topal, B., Gokceoglu, C., Ozcan, A., Erbasli, C., Cebeloglu, F. S., Koruyucu, M., and Binal, B. E.: Performance Comparison of Some Artificial Intelligence Algorithms for Metallic Mineral Deposits: A Case from Türkiye, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20311, https://doi.org/10.5194/egusphere-egu26-20311, 2026.

EGU26-20838 | ECS | Orals | GI2.1

AI-Based Quantification of Crack Geometry on Retaining Walls from Mobile Earth-Observation Imagery 

Yen-Chun Chiang, Shao-Chin Chu, and Guan-Wei Lin

Cracks on retaining walls and road surfaces can reveal the early warning signs of geohazards such as landslides or slumps in rural areas. However, even today, many governments still rely on manual visual inspection to identify and evaluate cracks, which is time-consuming, subjective, and highly dependent on individual experience. Artificial intelligence (AI) applied to Earth-observation imagery not only enables the detection of potentially dangerous cracks but also makes it possible to quantify their geometric properties, providing a more objective and quantitative basis for infrastructure monitoring and geohazard risk management.

Nevertheless, several key challenges remain. First, although recent studies have developed many advanced algorithms for crack detection and segmentation, methods for measuring crack width, length ,and area are still insufficient. Second, most existing models are designed for road cracks, while cracks on retaining walls present more complex textures, illumination conditions, and background noise, requiring dedicated model fine-tuning. Third, in regions with dense vegetation, branches, leaves, and shadows often produce false detections, making it difficult for AI models to distinguish real cracks from environmental interference.

In this study, we aim to quantify crack geometry from mobile panoramic Earth-observation imagery and to develop an AI model optimized for cracks on retaining walls in complex environments. A multi-stage approach is used to combine YOLO-based crack detection with 3D geospatial information for estimating the length, width, and area of individual cracks. By focusing on real cracks under vegetation-rich and noisy conditions, this approach advances AI-based quantitative analysis of surface degradation. These crack metrics provide a foundation for future retaining wall stability assessment and risk-informed infrastructure management.

How to cite: Chiang, Y.-C., Chu, S.-C., and Lin, G.-W.: AI-Based Quantification of Crack Geometry on Retaining Walls from Mobile Earth-Observation Imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20838, https://doi.org/10.5194/egusphere-egu26-20838, 2026.

EGU26-22777 | Posters on site | GI2.1

AETHER: AI Enhancement for Third-gen Earth observing ImageR. Reaching 3x spatial upsampling and 10x temporal upsampling from existing MTG-I products. 

Nicolas Dublé, Sylvain Tanguy, Lucas Arsene, Vincent Poulain, Danaele Puechmaille, Oriol Hinojo Comellas, and Miruna Stoicescu

The Meteosat Third Generation (MTG) mission represents a major step forward in geostationary meteorological observation by combining, onboard Meteosat-12, multiple instruments with highly complementary characteristics. Among them, the Flexible Combined Imager (FCI) provides multispectral images of the full Earth disk every ten minutes with a spatial resolution reaching 1 km at nadir, while the Lightning Imager (LI) observes the same scene at a much higher temporal sampling, but with a coarser spatial resolution of approximately 4.5 km at nadir. Although designed for distinct operational purposes, these two sensors offer a unique opportunity for joint exploitation, as they observe identical atmospheric phenomena under fundamentally different spatio-temporal trade-offs. In this context, Thales investigates the use of artificial intelligence techniques to leverage this complementarity and generate enhanced observation products from existing MTG-I data. 

The core hypothesis of this work is that the high temporal density of LI observations implicitly encodes fine-scale spatial information. In other words, temporal correlations within LI time series can partially compensate for the sensor’s lower spatial resolution. By exploiting these correlations, fine spatial features can be reconstructed from high temporal frequencies. The availability of reference matching high resolution data enables to consider this process without the need for artificially degraded training data. 

To implement this hypothesis, a hybrid deep learning architecture combining convolutional neural networks (CNNs) and Transformers is proposed. CNN components are used to efficiently extract local spatial structures, such as gradients, cloud edges, and internal texture patterns, while Transformer-based attention mechanisms model short- and long-range temporal dependencies across successive LI acquisitions. This combination enables a joint representation of spatial detail and temporal coherence, while remaining compatible with large data volumes and near-operational processing constraints. 

The proposed approach is evaluated along two complementary scientific tasks. The first focuses on spatial super-resolution of LI images using LI temporal sequences alone. The second addresses the fusion of FCI and LI data to generate a product combining high spatial resolution with high temporal frequency. In both cases, the results are conclusive. The use of FCI images as a cross-reference makes it possible to assess the physical consistency of reconstructed features and to prevent the introduction of spurious, non-physical details. The super-resolved products remain radiometrically consistent with the input observations, with low radiance discrepancies (RMSE below 1), while recovering finer spatial structures than those achievable through conventional interpolation methods. Compared to standard SISR (Single Image Super Resolution), CNN + Temporal Conv1D, CNN + sparse Conv3D approaches, the hybrid CNN–Transformer model achieves the best overall performance. 

As a perspective, the proposed method shows strong potential for operational deployment. Its computational efficiency allows approximately one hour of MTG data—corresponding to about sixty full-disk Earth images—to be processed in less than five minutes on standard computing infrastructure with one Nvidia H-100 configuration, paving the way for the routine generation of high-resolution, high-frequency products from existing geostationary missions. 

How to cite: Dublé, N., Tanguy, S., Arsene, L., Poulain, V., Puechmaille, D., Hinojo Comellas, O., and Stoicescu, M.: AETHER: AI Enhancement for Third-gen Earth observing ImageR. Reaching 3x spatial upsampling and 10x temporal upsampling from existing MTG-I products., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22777, https://doi.org/10.5194/egusphere-egu26-22777, 2026.

EGU26-254 | Posters on site | GI2.2

Seeing the Winds Better: Simulated Videos of Defoliated Tree Motion Capture Extreme Wind Speeds 

Sai Kulkarni, John K. Hillier, Sarah L. Bugby, Timothy I. Marjoribanks, Daniel Bannister, and Jonny Higham

Extreme windstorms are among the costliest natural disasters in northwest Europe. Traditional wind measurement methods, while reliable, are limited by cost, installation complexity, and sparse spatial coverage, particularly in cluttered urban areas. Higher resolution approaches are therefore needed to monitor near-surface wind dynamics in complex settings.

Motion tracking in videos of foliated trees has reliably captured fine-scale wind variability, showing strong correlations with anemometer measurements, consistent gust estimates across reference objects, and strong temporal coherence; the present work introduces two major advances: (1) the first application of Visual Anemometry (VA) on videos generated from physics-based simulations of trees, and (2) a focus on defoliated trees, enabling mechanistic isolation of branch and trunk responses. Videos are generated from an elastically articulated body model simulating tree responses under mean wind speeds of 7-40 m s⁻¹ (25-144 km h⁻¹).

Results show that input wind speeds are reflected in kinematic tree responses ( = 0.8), and then that these tree motions are captured in wind speeds estimated from videos by VA (≈ 0.7). Distal and mid-canopy branches dominate the VA response, whereas the stem and inner branches provide only weak contributions, even though informative motion cues may occur anywhere in the canopy. These VA wind estimates were insensitive to camera orientation, confirming that estimation accuracy remains robust across horizontal viewpoints. In this work, we also explore the method's sensitivity to different camera parameters and assess its transferability across different conditions.

Using simulation-based defoliated trees, this work is a step towards a low-cost, scalable alternative to traditional methods, enabling improved detection of extreme gusts, fine-scale hazard mapping, and risk assessment for urban planning and insurance.

How to cite: Kulkarni, S., Hillier, J. K., Bugby, S. L., Marjoribanks, T. I., Bannister, D., and Higham, J.: Seeing the Winds Better: Simulated Videos of Defoliated Tree Motion Capture Extreme Wind Speeds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-254, https://doi.org/10.5194/egusphere-egu26-254, 2026.

EGU26-1694 | Posters on site | GI2.2

Spruce and Peatland Responses Under Changing Environments (SPRUCE) - 10 years of data collection 

Misha Krassovski, Melanie Mayes, Terri Velliquette, Tom Ruggles, Paul Hanson, and Jeff Riggs

The SPRUCE experiment is the primary component of the Terrestrial Ecosystem Science Scientific Focus Area at ORNL focused on terrestrial ecosystems and the mechanisms that underlie their responses to environmental change. As of December 2025, the SPRUCE experiment is ending its planned decadal timeframe. The manipulation evaluated the response of the existing biological communities to a range of warming levels from ambient to +9°C, provided via large, modified open-top chambers. The ambient and +9°C warming treatments were also conducted at eCO2 (in the range of 800 to 900 ppm). Both direct and indirect effects of these experimental perturbations have been analyzed to develop and refine models needed for full Earth system analyses. The instruments and infrastructure needed for these measurements include meteorological tower-based CO2/H2O sampling and analysis systems, air temperature and relative humidity probes, precipitation gauges, wind speed and direction instruments, solar radiation sensors, subsurface soil moisture and temperature sensors, water level and conductivity sensors, continuous vegetation sap flow and dendrometer sensors, and companion dataloggers to record and report the data. The data collection system deployed of approximately 80 dataloggers, 1100 sensors, and associated instruments. Through the 10 years of observations, we collected substantial amount of data and want to present variety of data product available for analysis and scientific investigation. 

How to cite: Krassovski, M., Mayes, M., Velliquette, T., Ruggles, T., Hanson, P., and Riggs, J.: Spruce and Peatland Responses Under Changing Environments (SPRUCE) - 10 years of data collection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1694, https://doi.org/10.5194/egusphere-egu26-1694, 2026.

High spatiotemporal monitoring of near-surface precipitation phase (N-SPP) is essential for weather forecasting, transportation, agriculture, and hydrology. However, operational capability remains constrained as manual observations are being phased out, in situ surface instruments are sparse and often lack representativeness, and discrepancies persist between aloft phase estimates from radar/satellite and actual conditions at the ground. Recent studies have also reported an “upper-limit” effect in radar-based N-SPP products, further underscoring the need for low-cost, automated, and scalable alternatives.

Urban surveillance cameras are ubiquitous in modern cities and continuously capture near-surface scenes at high temporal resolution. As precipitation particles traverse the camera field of view, the resulting videos inherently preserve rich visual–temporal signatures of hydrometeors, providing a viable basis for visually discriminating precipitation phases. Moreover, leveraging existing camera infrastructures requires no dedicated sensor deployment, making camera sensor networks a cost-effective solution for high-resolution N-SPP monitoring. Nevertheless, reliably distinguishing common N-SPP types (i.e., rain, snow, and graupel) in unconstrained videos remains challenging due to subtle inter-class differences and strong sensitivities to illumination changes, complex backgrounds, camera settings, and wind-driven trajectories.

Our previous study (Wang et al., 2025) demonstrated the feasibility of using urban surveillance cameras for N-SPP monitoring. Guided by meteorological, optical, and imaging principles, we identified discriminative cues from both daytime and nighttime videos and developed an efficient framework that couples MobileNetV2-based transfer learning for spatial feature extraction with GRU-based temporal modeling. Using a self-curated 94-hour surveillance video dataset and benchmarking against 24 baseline methods, the proposed approach achieved the best overall performance, with accuracies of 0.9677 on the dataset and 0.9301 in real-world field validation against manually quality-controlled 2DVD measurements. The model also remained stable under variations in camera settings and across day–night conditions, and exhibited satisfactory wind robustness for wind speeds below 5 m/s.

Building on these results, we further move toward operational, city-scale deployment by discussing key challenges in multi-camera collaborative observing, including camera siting and field-of-view geometric constraints, automated camera screening and tiered selection, and quality-control/anomaly-detection procedures to address occlusion, glare, raindrop adhesion or wiper interference, stream frame loss, and camera-parameter drift. These discussions provide practical guidance for constructing a stable and reliable surveillance camera–based N-SPP monitoring network.

 

Reference:

Wang, X., Zhao, K., Huang, H., Zhou, A., & Chen, H. (2025). Surveillance camera-based deep learning framework for high-resolution ground hydrometeor phase observation. Atmospheric Measurement Techniques Discussions, 2025, 1-38.

How to cite: Wang, X., Zhao, K., and Yang, Z.: Surveillance Camera Sensor Networks: An Emerging Observing System for Near-Surface Precipitation Phase Monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2076, https://doi.org/10.5194/egusphere-egu26-2076, 2026.

EGU26-3864 | Orals | GI2.2

Expansion of UFP measuring capabilities of the Dutch National Air Quality Monitoring Network 

Anneke Batenburg, Joost Wesseling, Dirk Wever, Sjoerd van Ratingen, Ernie Weijers, and Guus Stefess

The health effects of ultrafine particles (UFP) have come under increased scrutiny. In 2021, the Health Council of the Netherlands published the advisory report “Risks of ultrafine particles in the outside air”, which highlighted that our knowledge of UFP exposure and health effects is limited by a lack of structural measurements of UFP concentrations in the Netherlands. The report therefore recommended

  • measuring UFP concentrations structurally in the Dutch National Air Quality Monitoring Network and
  • performing structural and validated model calculations to obtain a national overview of UFP exposure.

At the subsequent request of the Ministry of Infrastructure and Water Management, RIVM made an inventory of available data, knowledge and measurement equipment, and developed integrated strategies for incorporating structural UFP measurements into the national network and improving UFP models.

The National Air Quality Monitoring Network currently performs indicative UFP measurements with three TSI EPC 3783 instruments. Diurnal and weekly cycles can already be observed in these indicative data, and they have been used to scale an updated empirical map of average UFP concentrations in the Netherlands as well. On a project base, short-term measurements of UFP are performed using more compact equipment.

Newer counting equipment (TSI CPC 3750-CEN10) has been purchased recently to perform stationary UFP concentration measurements according to the latest technical standard (EN 16976:2024). The locations where the new measurement equipment will be placed are selected with the specific aim to improve the yearly average concentration map and obtain better estimates for the exposure of the Dutch population to UFP. The data will be made available to the public.

This presentation will discuss the progress so far, first experiences with the new equipment and next steps, including steps required for compliance with the new EU Air Quality Directive.

How to cite: Batenburg, A., Wesseling, J., Wever, D., van Ratingen, S., Weijers, E., and Stefess, G.: Expansion of UFP measuring capabilities of the Dutch National Air Quality Monitoring Network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3864, https://doi.org/10.5194/egusphere-egu26-3864, 2026.

EGU26-4030 | Orals | GI2.2

From rapid assessment to real-time warning: short-term rockfall monitoring along the Route d’Anniviers (Valais, Switzerland) 

stéphane vincent, maxence carrel, theo st.pierre, jonas vonwartburg, olafur stitelmann, and janine wetter

From rapid assessment to real-time warning: short-term rockfall monitoring along the Route d’Anniviers (Valais, Switzerland)

 

The Val d’Anniviers is one of the major valleys of the canton of Valais in Switzerland. Well known for its winter sports opportunities and for the villages of Grimentz and Zinal, the valley is accessible by a vertiginous road exposed to a wide range of gravitational hazards. Though the Route d’Anniviers is protected by multiple galleries, severe events can still impact the road.In March 2024, a series of rockfalls led to heavy accumulation of debris atop a road gallery at the entrance of the valley. A week later, on 29 March, bigger blocks hit the road and perforated the gallery. To avoid complete isolation, an alternative route estimated to be less safe was used from the other side of the valley. In this context, real-time monitoring became essential to support decision-making and rapid response during emergency operations and gallery rehabilitation. A first emergency phase focused on rapid assessment: Geoprevent was mandated by the local authorities to deploy an interferometric radar to monitor and accurately assess the area above the Croisettes sector (near Vissoie) and check whether significant movement was ongoing. Early observations suggested only limited changes. This initial phase helped establish shared situational awareness and informed the next steps toward an operational warning setup. An alarm system was then needed to be installed to increase the safety of workers during the gallery renovation, as well as to contribute to a longer-term mitigation plan. Geoprevent was mandated on 10 April by the local authorities and installed a rockfall Doppler radar on 22 April. This technology enables real-time detection of rockfall activity. The radar was coupled with traffic lights and alarm horns, allowing rapid road closure and immediate on-site warning in case of events. SMS and email alerts complement local signaling, and both radar data and live footage from a pan-tilt-zoom remotely controllable camera are available through Geoprevent’s online data portal for remote supervision and event review. This contribution  presents the phased monitoring and warning approach implemented at Vissoie—from rapid assessment to operational warning system —and discusses lessons learned for short-term monitoring, emergency installation, data interpretation, and reliable alerting to insure road and people safety in a complex environment.

How to cite: vincent, S., carrel, M., st.pierre, T., vonwartburg, J., stitelmann, O., and wetter, J.: From rapid assessment to real-time warning: short-term rockfall monitoring along the Route d’Anniviers (Valais, Switzerland), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4030, https://doi.org/10.5194/egusphere-egu26-4030, 2026.

EGU26-4108 | Posters on site | GI2.2

The In-situ Sensing Facility: Agile Observation Networks for Field Campaign Success 

Jacquelyn Witte, William Brown, Holger Vömel, Christopher Roden, Sebastian Hoch, and Terry Hock

The National Center for Atmospheric Research (NCAR), funded by the US National Science Foundation, has been supporting field deployments for atmospheric research since the 1960s, with its Earth Observing Laboratory (EOL) coordinating large-scale programs. EOL’s In-situ Sensing Facility (ISF) was forged out of decades of instrument development, advances in technology and software, and an evolution of services and support in response to the changing landscape of research. Today, ISF has evolved into three measurement systems: (1) Airborne Vertical Atmospheric Profiling System - dropsonde technology, (2) Integrated Sounding System - combined in-situ and remote ground-based profiling instruments, and (3) Integrated Surface Flux System - suite of mesonet, turbulence and energy balance sensors mounted on scalable towers. These requestable observing systems are designed for scalability and flexibility, emphasizing sensor development and integration, data management, and robust deployments to remote or challenging locations. Observations from ISF's measurement systems have guided regional model and forecast development, supported boundary layer meteorology and turbulence studies, and enhanced our understanding of severe weather and convective processes. When configured together ISF forms the foundation of LOTOS (Lower Troposphere Observing System) - a proposed sensor network to sample fundamental state parameters vertically through the boundary layer and horizontally across the surrounding landscape to provide a wealth of data to advance process studies and model algorithm development. We present an overview of our facilities' instrument capabilities and the LOTOS concept. 

How to cite: Witte, J., Brown, W., Vömel, H., Roden, C., Hoch, S., and Hock, T.: The In-situ Sensing Facility: Agile Observation Networks for Field Campaign Success, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4108, https://doi.org/10.5194/egusphere-egu26-4108, 2026.

EGU26-4925 | ECS | Posters on site | GI2.2

A Dual-Mode Expansion Cloud Chamber for Reproducible Laboratory Studies of Laser Propagation in Fog and Clouds 

Thomas Kociok, Kathrin Kociok, Dirk Seiffer, and Karin Stein
In this paper, we present the development of a portable expansion cloud chamber designed to investigate the interaction of high-power laser radiation (≥ 3 kW) with fog and cloud structures under controlled and reproducible laboratory conditions. The main aspects of the facility design, operating principles, and achievable atmospheric parameter ranges are discussed, with particular emphasis on controlled cloud and fog generation and optical propagation experiments.
The chamber employs a dual-mode adiabatic expansion concept, allowing both gradual pressure reduction using vacuum pumps and rapid decompression via a secondary pressure reservoir. This approach enables precise control of supersaturation conditions and reproducible formation of fog and cloud fields through controlled decompression.
The main chamber consists of a double-walled cylindrical vacuum vessel with an internal diameter of 2 m and a length of 10 m, integrated into a 45-foot container structure. The system covers a wide operational parameter space, including temperatures from −50 °C to +40 °C, relative humidity from 0 % to 100 %, and pressures between 100 and 1100 mbar. Homogeneous air mixing is achieved using multiple fan configurations, while configurable heating elements allow the generation of turbulent flow regimes. A dense and redundant sensor network provides real-time monitoring of thermodynamic, microphysical, and optical parameters at multiple locations within the chamber.
This experimental setup enables fundamental investigations of laser propagation, attenuation, and scattering in realistic atmospheric conditions. The facility provides a controlled platform for advancing the understanding of laser–atmosphere interactions and supports the development and validation of optical propagation models, with direct relevance for free-space optical and satellite communication systems.

How to cite: Kociok, T., Kociok, K., Seiffer, D., and Stein, K.: A Dual-Mode Expansion Cloud Chamber for Reproducible Laboratory Studies of Laser Propagation in Fog and Clouds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4925, https://doi.org/10.5194/egusphere-egu26-4925, 2026.

EGU26-5380 | ECS | Posters on site | GI2.2

Applicability of self-consistency calibration method for polarimetric cloud radars 

Renju Nandan and Christine Unal

Cloud radars are powerful tools for investigating cloud formation, radiative processes, and cloud microphysics. In recent years, polarimetric cloud radars have become increasingly common around the world. Since many cloud property retrieval techniques rely on accurately measured reflectivity, ensuring high-quality calibration is essential. The most widely used calibration approach is one based on disdrometer measurements, but this method carries significant uncertainties, particularly due to the vertical variability of rainfall characteristics. Another conventional method is the one based on point target observations, i.e. using hard targets such as corner and sphere reflectors (Toledo et al.,2020), but it is work intensive and difficult to carry out. Another method is the calibration transfer of a radar to those that are not calibrated yet (Jorquera et al.,2023) for e.g. BASTA radar in CCRES. The main disadvantage of the calibration transfer method is the high time consumption. Since the time needed to ship the reference radar to each location and carrying out the calibration is high, in a year maximum 2 or 3 radars can be calibrated. Another method of calibration is by comparison of observations by ground-based cloud radars and space-borne W-band radars in CloudSat and EarthCARE. EarthCARE (CloudSat) flight cycle of 25 (16) days and the requirement in pure ice nonprecipitating clouds during an overpass, makes this method mainly applicable for long-term calibration monitoring. To address all these limitations and complement in cloud radar calibration methods, A. Myagkov et al. (2020) introduced a self-consistency calibration technique that makes use of the polarization capabilities of W-band cloud radars. In this study, we assess the suitability of the self-consistency calibration method and identify the modifications required to make the approach more user-friendly and practical for operation.For this study, we have used 94 GHz cloud radar data operated at 300 elevation angle during days having rainfall rate less than 20 mm/hr. The methodology of self-consistency method consists of 4 steps. 1) Using Rayleigh Plateau detection method (Unal and van den Brule,2024), retrieve propagational (Kdp) and backscattering (δ) components from differential phase (φ) and, differential attenuation (Adp). 2) Calculate non-attenuated reflectivity Z0. 3) Calculate Kdp and Adp using Z0, δ and the coefficients given in A. Myagkov et al. (2020). 4) Compare the measured and calculated Kdp and Adp, and find the best fit for calibration coefficient.The major findings of this study are summarized as follows:1) A 30° elevation angle and rainfall rate below 20 mm/hr are not the only criteria required for applying the self-consistency method. The values of differential backscatter phase(δ) and Doppler spectrum width also play important roles. 2) The influence of surface temperature on the method has been examined.3)The criteria for selecting suitable cloud radar observations for the self-consistency calibration approach have been clearly identified.4)In addition to the calibration of reflectivity, the retrieval of the one-way attenuation profile is shown to be another significant output of the self-consistency calibration technique.

 

 

 

How to cite: Nandan, R. and Unal, C.: Applicability of self-consistency calibration method for polarimetric cloud radars, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5380, https://doi.org/10.5194/egusphere-egu26-5380, 2026.

EGU26-5857 | ECS | Posters on site | GI2.2

Global evaluation of Pandonia Global Network total column water vapour using co-located AERONET and GRUAN observations 

Dan Weaver, Xiaoyi Zhao, Thomas Frost Hanisco, Pawan Gupta, Alexander Cede, Martin Tiefengraber, Manuel Gebetsberger, and Michael Sommer

Improving measurements of atmospheric water vapour remains a priority for the atmospheric science community, including for evaluation of satellite retrievals. The Pandonia Global Network (PGN) provides long-term, high-temporal-resolution direct-sun observations of total-column water vapour at many sites worldwide, but the PGN H2O product has not yet been widely assessed against independent ground-based datasets across diverse conditions.

Here we present preliminary intercomparisons of PGN total-column water vapour with coincident AERONET sun-photometer retrievals at co-located sites, with additional context from comparisons to GRUAN-processed radiosonde profiles where available. We examine sensitivities to temporal matching and to factors such as solar zenith angle, season, and humidity regime and report initial network-wide and site-to-site statistics (bias, scatter, correlation).

How to cite: Weaver, D., Zhao, X., Hanisco, T. F., Gupta, P., Cede, A., Tiefengraber, M., Gebetsberger, M., and Sommer, M.: Global evaluation of Pandonia Global Network total column water vapour using co-located AERONET and GRUAN observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5857, https://doi.org/10.5194/egusphere-egu26-5857, 2026.

In situ atmospheric particulate matter (PM) monitoring networks play a critical role in advancing understanding of air quality dynamics across local to regional scales by providing continuous, site-resolved observations. In contrast to short-term measurement campaigns, sustained monitoring networks enable the characterization of long-term trends, episodic events, and source-specific variability, while providing essential data for model validation and exposure assessment. These capabilities are especially useful in industrial environments, where emissions are spatially heterogeneous, temporally variable, and chemically complex.

We present the design and implementation of the Environmental Monitoring for Industrial Sites (ÉMIS) network, a ground-based, distributed system developed to monitor complex industrial emission environments. The network is designed to operate under challenging conditions, including high-latitude environments with extreme seasonal variability, limited access to grid power, and constrained connectivity. Each station integrates measurements of particulate matter across multiple size fractions (PM2.5, PM5, and PM10) and volatile organic compounds using low-cost optical sensors, local meteorology, and visual documentation via a conditionally triggered camera. Stations are additionally equipped with a modified Wilson and Cooke (MWAC) bottle sampler to collect long-term, sector-representative samples for chemical characterization.

Stations transmit data using long-range radio (LoRa) at user-defined intervals (e.g., two-minute resolution) to a hub node, which aggregates and relays data via cellular or satellite communication to an online dashboard. Unlike Bluetooth or Wi-Fi, LoRa enables kilometer-scale data transmission without the cost or infrastructure requirements of cellular modems. This architecture provides near–real-time insight into emission dynamics while supporting long-term data continuity. Emphasis on low-cost, modular instrumentation reduces financial and logistical barriers associated with traditional monitoring systems, enabling high-density deployments accessible to researchers, industries and public stakeholders.

The initial field deployment consisted of fifteen (15) stations distributed across a copper smelter in Quebec, Canada, spanning more than 1 km². This case study demonstrates the network’s ability to resolve spatial gradients and localized emission signals, while dealing with complex topography and climate conditions. Analysis reveals persistent PM hotspots associated with heavy machinery traffic, ore handling operations, and slag cooling. Periodic PM spikes linked to train transport, as well as clear relationships between wind speed, wind direction, and plume occurrence were identified.

The multi-level data output from the ÉMIS network supports a wide range of applications, including PM source attribution, evaluation of emission dynamics, integration with receptor and dispersion modeling, and validation of satellite-derived products. The network also serves as a testbed for sensor development, quality assurance refinement, and cross-network harmonization under real-world industrial conditions. This work highlights how adaptable, cost-effective ground-based monitoring networks can expand observational capacity in industrial environments and support advances in atmospheric science, air-quality management, and community-informed decision-making.

How to cite: King, J., Norris, E., and Hayes, P.: Environmental Monitoring for Industrial Sites (ÉMIS): A Distributed LoRa-based Network for Real-Time Particulate Matter Characterization in Complex Environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13103, https://doi.org/10.5194/egusphere-egu26-13103, 2026.

EGU26-13621 | Orals | GI2.2

Preliminary Design of a Passive System for Monitoring Volcanic Emissions Exploiting Microwave GEO Satellite Downlinks  

Filippo Giannetti, Emanuele Maria Sciortino, Ottavia Gherardini, Fabiola Sapienza, and Alessandro Piras

Opportunistic sensing based on microwave satellite downlinks has recently gained attention as a cost‑effective approach for monitoring tropospheric phenomena, exploiting the attenuation experienced by communication signals as they propagate through the atmosphere. While this approach has been successfully applied to meteorological phenomena—particularly rainfall estimation using Ku‑band broadcasting links and, more recently, Ka‑band broadband services—its use for geophysical monitoring remains largely unexplored.  Volcanic emissions, in particular, release atmospheric constituents capable of significantly affecting microwave propagation through absorption and scattering, depending on particle size, concentration, and chemical composition. In regions surrounding active volcanoes, the interaction between ash, gases, and microwave signals offers an opportunity to detect eruptive activity using low‑cost ground receivers.

This work investigates the feasibility of using commercial satellite downlink signals to sense volcanic emissions in real time. The analysis considers the general interaction between microwave signals and volcanic constituents and examines how the Ku‑ and Ka‑band frequencies commonly used by GEO satellites provide different levels of sensitivity to these atmospheric components. Since these signals are continuously available over wide areas, they offer an attractive resource for passive and inexpensive monitoring.

A key aspect in assessing the feasibility of such opportunistic sensing is the geometry of the satellite–receiver link, which strongly influences the detectability of volcanic emissions. As matter of fact, the relative position of the satellite, the ground station, and the volcanic plume determines whether the microwave path intersects the cloud and at which altitude and distance from the vent this intersection occurs. In volcanic regions such as Mount Etna (Italy), the simultaneous visibility of multiple GEO satellites at different azimuths and elevations increases the likelihood that at least one downlink path crosses the plume, enabling the detection of its impact on the received signal.

This preliminary study provides thus a first assessment of the geometric and physical conditions under which satellite downlink signals can be exploited for volcanic emission detection.

The results suggest that existing broadcast satellite infrastructure could be leveraged also as a low‑cost, wide‑area monitoring system, complementing conventional geophysical instruments and motivating future experimental validation.

Acknowledgements: This work was supported by the following projects: Space It Up, funded by Italian Space Agency (ASI) and the Italian Ministry of University and Research (MUR) – Contract 2024-5-E.0 - CUP I53D24000060005; FoReLab (Departments of Excellence), funded by MUR.

How to cite: Giannetti, F., Sciortino, E. M., Gherardini, O., Sapienza, F., and Piras, A.: Preliminary Design of a Passive System for Monitoring Volcanic Emissions Exploiting Microwave GEO Satellite Downlinks , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13621, https://doi.org/10.5194/egusphere-egu26-13621, 2026.

EGU26-13828 | Posters on site | GI2.2

The Quantum Gravimeter Network of the Canary Islands 

Luca D'Auria, Nemesio M. Pérez, Aarón Álvarez-Hernández, Sergio de Armas-Rillo, Rubén García-Hernández, Pablo López-Díaz, David M. van Dorth, Víctor Ortega-Ramos, Paul Bertier, Laura Faure, Romain Gautier, and Jérémie Richard

The island of Tenerife (Canary Islands) exhibits the highest volcanic risk in Spain, owing to its long volcanic history combined with high population density. Consequently, an effective volcanic early-warning system is essential to ensure the safety of both the island’s residents and the millions of tourists who visit each year. Tenerife already hosts one of the most advanced volcano monitoring programs worldwide, integrating permanent instrumental networks with periodic geophysical and geochemical surveys.

Continuous microgravity measurements have proven to be a sensitive and reliable tool for detecting changes in magmatic–hydrothermal systems that may remain undetected by other geophysical or geochemical techniques [1]. However, spring-based gravimeters are affected by instrumental drift, which can compromise the interpretation of long-term observations. Superconducting gravimeters, while offering the highest sensitivity, require complex liquid helium refrigeration systems, significantly limiting their operational deployment. In recent years, absolute quantum gravimeters have emerged as the state-of-the-art technology for microgravity monitoring [2]. Time series acquired at active volcanoes, such as Mount Etna [3], demonstrate that these instruments can detect and quantify subsurface mass redistributions associated with volcanic processes. Within the framework of the GEOFIS-CAN project, the Instituto Volcanológico de Canarias (INVOLCAN) has acquired three Exail AQG-A absolute quantum gravimeters to be deployed on Tenerife.

The volcanic system of Tenerife consists of a central caldera (Las Cañadas), which hosts the Teide–Pico Viejo volcanic complex and is characterized by both basaltic and phonolitic activity, and three radial dorsals dominated by fissural basaltic effusive eruptions. The central complex, as well as the northwestern (NW) and northeastern (NE) dorsals, have experienced eruptions within the last 500 years. The three AQG instruments will be installed at: (1) the NW dorsal (Santiago del Teide), the most volcanically active sector of the island; (2) the boundary between the Las Cañadas caldera and the NE dorsal (Izaña); and (3) the southern margin of the caldera (Vilaflor). This network geometry provides comprehensive coverage of all regions potentially affected by future eruptions. Moreover, it enables not only the detection but also the localization of subsurface mass changes within the volcanic edifice. Specifically, this configuration is sufficient to simultaneously and unambiguously constrain both the location and magnitude of the mass variations within the volcanic edifice.

In this work, we present a sensitivity analysis of the proposed gravimetric network configuration, together with preliminary results from the recorded dataset.

 

References

[1] de Zeeuw-van Dalfsen, E., & Poland, M. P. (2023). Microgravity as a tool for eruption forecasting. Journal of Volcanology and Geothermal Research, 442, 107910.

[2] Ménoret, V., Vermeulen, P., Le Moigne, N., Bonvalot, S., Bouyer, P., Landragin, A., & Desruelle, B. (2018). Gravity measurements below 10− 9 g with a transportable absolute quantum gravimeter. Scientific reports, 8(1), 12300.

[3] Antoni‐Micollier, L., Carbone, D., Ménoret, V., Lautier‐Gaud, J., King, T., Greco, F., ... & Desruelle, B. (2022). Detecting volcano‐related underground mass changes with a quantum gravimeter. Geophysical Research Letters, 49(13), e2022GL097814.

How to cite: D'Auria, L., Pérez, N. M., Álvarez-Hernández, A., de Armas-Rillo, S., García-Hernández, R., López-Díaz, P., M. van Dorth, D., Ortega-Ramos, V., Bertier, P., Faure, L., Gautier, R., and Richard, J.: The Quantum Gravimeter Network of the Canary Islands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13828, https://doi.org/10.5194/egusphere-egu26-13828, 2026.

Computing power network (CPN) is designed to utilize multi-dimensional resources to complete computing tasks. However, in practical applications, the CPN architecture has difficulty in coordinating cross-domain heterogeneous resources, making it impossible to achieve the real-time and high scalability requirements of computationally intensive and time-sensitive tasks such as levee piping hazard inspection via remote sensing in emergency scenarios. Based on this, we propose a communication and computation integrated network architecture, referred to as (Com)2INet, that integrates “sensing”, “transmission”, and “computation” phases. In the sensing phase, thermal infrared imagery is utilized to retrieve land surface temperature fields through radiative transfer mechanisms, providing a reliable foundation for visual segmentation of piping hazards. In the transmission phase, we adopt the designed multi-path transmission mechanism to promote the efficient data flow across heterogeneous networks. In the computation phase, the proposed SACM algorithm, which is functionally decomposed and implemented as service chains within the proposed network architecture, dynamically processes the retrieved temperature fields to achieve precise hazard identification. This integrated framework ensures seamless interaction between sensing, communication, and computation, addressing the challenges of real-time hazard detection in emergency scenarios.

How to cite: Chen, J.: Service-Chain-Driven Communication and Computing Integration Networking: A Case Study of Levee Piping Hazard Inspection via Remote Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15440, https://doi.org/10.5194/egusphere-egu26-15440, 2026.

EGU26-17517 | Posters on site | GI2.2

A Low-Cost Image-Based Monitoring System for Automatic Rock Displacement Measurement Using YOLO 

Ruoshen Lin, Michel Jaboyedoff, Marc-Henri Derron, Aubin Laurent, and Antonin Chalé

Accurate monitoring of rock movement is essential for understanding rock slope instability and early failure mechanisms. However, conventional monitoring techniques often rely on manual measurements or expensive instrumentation, limiting their practicality for continuous and large-scale deployment. This study presents a low-cost image-based monitoring system that enables fully automatic measurement of rock displacement using a YOLOv8 pose estimation model. The proposed system was evaluated at the Miroir d’Argentine rock wall, a limestone rock flake in the Swiss Alps, Switzerland, using image data acquired from a Futuro BRW comparator monitored by a low-cost digital camera. The model was trained to detect the manual dial indicator and estimate pointer positions, allowing rock displacement to be derived automatically from pictures without manual intervention. To further assess the practical applicability of the proposed system, additional images acquired at different time periods were used for independent validation. The results demonstrate that the proposed approach can reliably estimate rock movement with high accuracy and strong generalization capability under real-world conditions. In addition, the robustness of the method was evaluated under simulated fog and blur degradations. The results show that the system maintains stable performance under light to moderate visual degradation, while performance decreases under severe fog and strong motion blur due to reduced geometric visibility. Overall, the proposed method provides an effective, low-cost, and practical solution for continuous rock movement monitoring and shows strong potential for long-term deployment in challenging alpine environments.

How to cite: Lin, R., Jaboyedoff, M., Derron, M.-H., Laurent, A., and Chalé, A.: A Low-Cost Image-Based Monitoring System for Automatic Rock Displacement Measurement Using YOLO, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17517, https://doi.org/10.5194/egusphere-egu26-17517, 2026.

EGU26-18236 | Posters on site | GI2.2

Removal of temperature drift from tiltmeter recordings 

Stella Pytharouli and Chenchen Qiu

MEMS Tiltmeters are an effective tool in high-precision monitoring of ground and infrastructure but their sensitivity to temperature variations remains a challenge. This can be a prohibiting factor for their application in field monitoring of natural processes, despite the fact that tiltmeters are likely one of the very few technologies that can provide information on minute movements in real-time and at relatively low cost. Temperature drift, if not removed effectively, can completely mask small tilts or lead to wrong interpretations of the monitored process. Up until very recently, the tiltmeter response to temperature change was assumed to be instantaneous, but previous work by the authors has shown that there is a delay of varying duration between the two over time. We present a weighted least square (WLS) - based method that takes this dynamic change of time-lags into consideration. The time-series data is divided into a number of time-windows based on time-lag values, wherein windows with identical lags are grouped together. Time windows longer than a specified duration are subdivided based on an optimal window length. We describe a method for selecting the optimal window size applicable to different monitoring scenarios. Finally, an iteratively WLS is applied to produce values that best represent the temperature drift over time within each time window. To examine the impact of varying window sizes on results, a sensitivity analysis is performed using the Monte Carlo method, enabling the calculation of prediction intervals. Our approach provides a reliable framework for the removal of temperature drift from tiltmeter recordings, enabling the use of tiltmeters for the monitoring of subtle ground movements. This can be crucial for applications such as early warning systems for landslides and monitoring of the ground surface response to hydrological processes at depth.

How to cite: Pytharouli, S. and Qiu, C.: Removal of temperature drift from tiltmeter recordings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18236, https://doi.org/10.5194/egusphere-egu26-18236, 2026.

EGU26-20308 | Orals | GI2.2

Introducing a compact GC-PTR-TOF-MS: A novel method for the long-term monitoring of volatile organic compounds 

Megan Claflin, Urs Rohner, Vasyl Yatsyna, Brian Lerner, Augie Dobrecevich, Joel Thornton, Manjula Canagarantna, Felipe Lopez-Hilfiker, and John Jayne

Long-term, routine monitoring of volatile organic compounds (VOCs) is needed to provide insight into emission sources and patterns, oxidation processes including photochemistry and radical cycling, and the formation of tropospheric ozone and secondary organic aerosol. However, instrumentation that can provide high quality data both in terms of temporal resolution and molecular speciation has historically been cost-prohibitive, and requires advanced users for field deployment, operation, and data analysis.

While the use of proton transfer reaction mass spectrometry, paired with time-of-flight technology (PTR-TOF-MS), has been utilized for the detection of VOCs in a wide variety of environments and measurement platforms; this technique cannot provide molecular structure information and suffers from detection interferences such as fragmentation, cluster formation, and mixed ionization schemes that complicate data analysis and interpretation. Combining in situ gas chromatography (GC) with PTR-TOF-MS is a remedy, offering isomer level resolution and the ability to easily quantify product ion distributions to account for complex detection schemes. The addition of chromatographic pre-separation not only enhances the accuracy of species typically reported by PTR methods, it can also be used to broaden the scope of VOCs quantified using PTR methods, while maintaining low limits of detection (typically 1 ppt) without losing high time resolution data and negating the need for high mass resolving power.

Here, we present a new instrument package for the online, long-term detection of VOCs consisting of an in situ GC system equipped with an integrated thermal desorption (TD) system coupled to a compact PTR TOF-MS. The entire instrument is contained in a 50 x 65 x 55 cm footprint, weighs < 70 kg, and consumes < 600 W for typical operation. Coupling the GC system with the PTR-TOF allows the automated acquisition of both direct, high-time resolution data (e.g. 1 s) and pseudo-continuous molecular speciation data for isomer separation and improved quantification of the direct-PTR data.

A description of the instrument, including its utilization of a new VUV PTR ion source, will be presented along with > 4 weeks of continuous ambient data acquired in Spring 2025 in Thun, Switzerland. This data demonstrates the stability of the system and the value of continuous VOC detection with regular molecular speciation. This compact, easier to operate and maintain system makes it feasible to deploy this technology in many locations, including those with access limitations, for greater spatial resolution to acquire coinciding datasets to elucidate local, regional, and global VOC trends. 

The compact chemical ionization time-of-flight mass spectrometer (CI-TOF-MS) described, here utilizing proton transfer reaction (PTR) ionization, was developed with support from the Beckmann Foundation.

How to cite: Claflin, M., Rohner, U., Yatsyna, V., Lerner, B., Dobrecevich, A., Thornton, J., Canagarantna, M., Lopez-Hilfiker, F., and Jayne, J.: Introducing a compact GC-PTR-TOF-MS: A novel method for the long-term monitoring of volatile organic compounds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20308, https://doi.org/10.5194/egusphere-egu26-20308, 2026.

EGU26-20334 | ECS | Posters on site | GI2.2

Design and Implementation of a Low-Cost, Satellite-Enabled Environmental Data Logger 

Filippo Tagliacarne, Riccardo Valentini, and Francesco Renzi

Ground-based environment monitoring networks provide essential data for climate and air quality research. However, traditional monitoring infrastructure in remote areas often requires high upfront and operational costs. Satellite communication technologies offer a solution to reach these remote areas, but existing commercial systems frequently pair expensive data loggers with costly satellite transceivers, thus limiting their deployment potential. 

 

We present a novel satellite-enabled data logger designed to maximize compatibility while minimizing both purchase and operational costs. Our custom-designed Printed Circuit Board (PCB) combines data-logging and satellite transmission into a single unit, leveraging low-cost near-real-time bidirectional communication provided by the Astrocast CubeSat constellation. The integration approach helps reducing the hardware costs and the deployment complexity compared to traditional systems. 

 

The platform is built on an STM32L476 microcontroller (MCU) with 64 MB of internal memory and an integrated real-time clock (RTC), providing low-power operation essential for autonomous field deployments. The board is equipped with an atmospheric pressure sensor, an air temperature and relative humidity sensor, along with multiple communication interfaces for a flexible, sensor-agnostic architecture: UART, I²C, and ADC channels. This design allows seamless integration of different third-party environmental sensors such as atmospheric chemistry, hydrological monitoring or ancillary meteorological measurements, without requiring hardware modifications. 

 

The system pair the custom PCB with an Astronode S module for satellite data transmission, enabling bidirectional data transmission with 2-3 transmission opportunities every day. The design provides extended operational autonomy through low-power management while maintaining regular access to measurement throughout Astrocast's API and web UI. 

 

We demonstrate how this design advances the objectives of ground-based monitoring networks by: (1) reducing deployment barriers to remote monitoring through cost-effective satellite connectivity, (2) supporting flexible sensor integration for cross-disciplinary measurement campaigns, (3) providing a scalable foundation for distributed monitoring networks, and (4) offering a validated, replicable platform for future infrastructure development.

How to cite: Tagliacarne, F., Valentini, R., and Renzi, F.: Design and Implementation of a Low-Cost, Satellite-Enabled Environmental Data Logger, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20334, https://doi.org/10.5194/egusphere-egu26-20334, 2026.

EGU26-20688 | ECS | Orals | GI2.2

One Researcher's Noise is Another's Signal: Dynamic Azimuthal Correction of ESCAT/ASCAT Backscatter for Long-Term Land Surface Monitoring 

Roland Lindorfer, Sebastian Hahn, Wolfgang Wagner, Clay T. Harrison, and Thomas Melzer

Satellite scatterometers are active radar instruments that transmit microwave pulses towards the Earth's surface and measure how much of this energy is reflected back, a quantity commonly referred to as backscatter. Operating at C-band, the ERS-1/2 ESCAT (1991–2011) and MetOp-A/B/C ASCAT (2007–present) missions together provide more than 35 years of global land surface backscatter observations. These data are widely used for monitoring soil moisture, vegetation dynamics, cryospheric processes, and land cover change. Their coarse spatial sampling of 12.5 km enables very high daily global coverage, which reaches about 82 % during the ASCAT era.

A characteristic feature of scatterometer measurements is azimuthal anisotropy, meaning that backscatter depends systematically on the viewing direction. This arises because ESCAT and ASCAT use multiple fixed fan-beam antennas that observe the same surface under different azimuth angles as the satellite passes overhead. Oriented surface structures such as vegetation patterns, agricultural rows, sand dunes, or wind-blown snow features (sastrugi), interact differently with the radar signal depending on their orientation relative to the radar look direction. While physically meaningful, this directional dependence introduces additional variability when measurements from different viewing geometries are combined, complicating the interpretation of collocated time series.

We present an updated azimuthal correction scheme for ESCAT and ASCAT backscatter that aims to improve the temporal consistency of long-term land surface monitoring. Earlier approaches relied on a unique static reference polynomial derived from multi-year data and mixed viewing geometries to implement the desired azimuthal bias correction, thereby harmonizing the data. Our updated method applies yearly reference polynomials instead and explicitly distinguishes between ascending and descending satellite orbits. This approach thus accounts for long-term land cover changes and systematic diurnal differences between morning and evening overpasses, which are preserved in the corrected backscatter. In addition, the right-looking satellite swath is used as the reference geometry, reflecting the single-swath configuration of the legacy ERS scatterometers. Consequently, this also supports a consistent alignment of measurements across diverse satellite missions. Global comparison maps and local examples show that the updated correction effectively reduces azimuthal noise, as indicated by a lower estimated standard deviation of the corrected backscatter. At the same time, genuine geophysical signals, such as systematic morning–evening differences likely linked to moisture variability, are preserved.

Azimuthal anisotropy is generally undesirable for most monitoring applications, as quantities such as soil moisture do not depend on viewing direction. However, we show that the correction polynomials themselves can provide useful information in specific environments, including sand dunes, ice sheets, and areas dominated by strong point scatterers. This can, for example, enable studies of the temporal migration of sand dunes or sastrugi. We also show that even individual buildings can affect the full footprint of a 25 km ASCAT pixel, as metal–glass structures can produce strong corner reflections when aligned with the radar look direction. The proposed approach therefore supports robust long-term monitoring of natural processes by reducing azimuthal noise, while the correction parameters themselves provide physically meaningful directional information.

How to cite: Lindorfer, R., Hahn, S., Wagner, W., Harrison, C. T., and Melzer, T.: One Researcher's Noise is Another's Signal: Dynamic Azimuthal Correction of ESCAT/ASCAT Backscatter for Long-Term Land Surface Monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20688, https://doi.org/10.5194/egusphere-egu26-20688, 2026.

EGU26-21164 | Posters on site | GI2.2

Comparison of TRACIS campaign data with data from radiosonde, IPRAL Lidar and ERA5 

Alexis Poignard, Antoine Farah, Alain Sarkissian, Philippe Keckhut, Dunya Alraddawi, Sergey Khaykin, Jean-Charles Dupont, and Julie Capo

The study of atmospheric composition is a major priority for improving the understanding of future climate models; therefore, it is essential to analyze in detail the variations of certain key variables, particularly water vapor, which strongly influences meteorological phenomena and plays a major role in radiative forcing. During my doctoral project, my research focused on studying the variability of water vapor using radiosoundings, an instrumental method for obtaining precise and high-quality measurements down to the UT/LS zone, by improving the quality of measurements through instrumentation. In addition to internal tests aimed at obtaining higher-quality measurements, setting up observation campaigns is a top priority in order to validate the performance of the sondes under real-world conditions, identify seasonal biases, and thus be able to make various corrections if necessary. Therefore, the TRACIS (Tropospheric Research Campaign on Air Moisture Content by Ipral at SIRTA) comparison campaign, in which I participated and which took place at the SIRTA site (Atmospheric Remote Sensing Research Instrumental Site) [48.71331°N, 2.20901°E] from May 12 to June 12, 2025, made it possible to assess the consistency of the data between the different sondes, while comparing these datasets with auxiliary sources such as ground-based observations and satellite measurements. This multi-source approach notably includes measurements from the IPRAL LiDAR, as well as fields from the ERA5 reanalysis model, thus strengthening the comparison, identifying potential systematic biases, and improving the overall interpretation of the results. Preliminary analyses focus on comparisons between the combined working measurement standard (CWS; mean RH M10/RS41) and other convergent datasets (M20, ERA5, and IPRAL LiDAR), allowing an evaluation of the representativeness and consistency of the different observation sources.

 

How to cite: Poignard, A., Farah, A., Sarkissian, A., Keckhut, P., Alraddawi, D., Khaykin, S., Dupont, J.-C., and Capo, J.: Comparison of TRACIS campaign data with data from radiosonde, IPRAL Lidar and ERA5, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21164, https://doi.org/10.5194/egusphere-egu26-21164, 2026.

Slow-moving landslides (SMLs) are governed by a combination of causative factors such as geology, tectonic setting, and climatic regime, along with triggering and conditioning factors including precipitation, complex groundwater dynamics, river toe erosion, seismic activity, and anthropogenic modifications. In this study, we present results from monitoring and analysis of a slow-moving landslide at Chandmari Village, Gangtok, in the eastern Himalaya. The analysis is based on real-world data obtained from an operational landslide early warning system active at the site since 2018. An integrated, multi-instrument dataset combining subsurface deformation measurements, hydro-meteorological observations, and high-resolution surface mapping is used to investigate landslide behaviour.

Slope movement was monitored using in-place inclinometer strings installed to depths of up to 30 m within the deforming slope mass to capture depth-wise displacement profiles. These measurements were analysed alongside continuous rainfall data recorded at 5-minute intervals from a local rain gauge to examine hydrological controls on deformation rates. In addition, Differential GPS (DGPS) surveys were conducted to map the spatial distribution of tension cracks on the slope surface. The combined dataset enabled assessment of both slip-surface depth and the spatial extent of the landslide body, as well as their response to seasonal rainfall.

Preliminary results indicate that periods of sustained rainfall correspond to increased displacement rates at specific depth intervals, suggesting activation of shear zones rather than a single, well-defined slip surface. Prolonged rainfall episodes further indicate the involvement of deeper slip surfaces. DGPS-based mapping reveals well-defined tension cracks at the head of the landslide body, while time-lag analysis between rainfall accumulation and deformation response highlights delayed slope adjustment controlled by groundwater dynamics.

The study demonstrates the temporal coupling between subsurface deformation and seasonal hydrological forcing and illustrates the effectiveness of multi-instrument monitoring for characterizing slow-moving landslides. The insights gained into deformation mechanisms support the development of improved early warning and mitigation strategies for urban hill-slope environments under long-term climatic and anthropogenic stress.

How to cite: Kumar M, N. and Vinodini Ramesh, M.: Integrated Analysis of Inclinometer, Rainfall, and DGPS Tension-Crack Data for a Slow-Moving Landslide: A Case Study from Chandmari Village, Sikkim, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21501, https://doi.org/10.5194/egusphere-egu26-21501, 2026.

EGU26-21819 | Posters on site | GI2.2

Copernicus Ground-Based Observations for Validation service (GBOV): overview and latest updates for EO data Cal/Val 

Christophe Lerebourg, Rémi Grousset, Simon Nativel, Jean-Sébastien Carrière, Marco Clerici, Nadine Gobron, Jan-Peter Muller, Rui Song, Jadu Dash, Somnath Paramanik, Finn James, Darren Ghent, Jasdeep Anand, Ritika Shukla, and Ana Perez-Hoyos

Copernicus Ground-Based Observations for Validation (GBOV) is a project funded by the European Commission and is part of the Copernicus Land Monitoring Service (CLMS). The project has two main purposes: to support yearly validation efforts of core CLMS products (BRF, Albedo, FAPAR, LAI, FCOVER, LST, Soil Moisture, GPP, NPP, LSP and Evapotranspiration), five of which are listed among GCOS Essential Climate Variables (ECV); and to maintain a data portal making these validation products available. GBOV has reached a broad user community, with about 1700 users, including ESA optical MPC.

A large number of ground-based measurement networks disseminate publicly available data such as NEON, ICOS, TERN, BSRN and ISMN. Within GBOV, long-term datasets are needed in order to maximise the number of matchups between ground-based measurements and satellite data.

GBOV produces both ground-based, point-scale observations (the so-called “Reference Measurements”), and Analysis Ready Validation Data (ARVD) which are spatially upscaled to match the resolution of CLMS products (the so-called “Land Products”). Those GBOV products cover more than 150 sites and are made available to the community via a data portal freely accessible on https://gbov.land.copernicus.eu/. Available Land Products variables include Surface Bi-directional Reflectance Factors (BRFs), Surface Albedo, Leaf Area Index (LAI), Fraction of Absorbed Photosynthetically Available Radiation (FAPAR), Fraction of Vegetation Cover (FCover), Land Surface Temperature (LST), Surface Soil Moisture (SSM). Gross Primary Production (GPP), Net Primary Production (NPP), Land Surface Phenology (LSP) and Evapotranspiration are new products and are not yet available, their release is planned for the end of 2026.

The networks providing GBOV initial input data are unfortunately not evenly distributed. In an attempt to reduce the thematic and geographical gaps, GBOV is developing its own network as part of a collaboration with existing networks. In GBOV phase 1, six ground stations have been upgraded with additional instrumentation. In GBOV phase 2, two ground stations monitoring vegetation variables have been deployed in 2023, one at the Fuji Hokuroku research station in Japan as part of a collaboration with NIES (National Institute of Environmental Studies) and one in 2024 at the Fontainebleau research station (France) as part of a GBOV/ICOS collaboration. In addition, two LST stations were deployed in Fuji Hokuroku and Litchfield (TERN network Australia) in 2024.

Over the past year, several updates have been implemented in the GBOV database to better respond to CLMS and general user requirements. This includes new procedures for specific land cover types in vegetation products, improved uncertainty estimates for soil moisture, and enhanced processing procedures for LST products. Procedures are being developed for the new products: Gross Primary Production, Net Primary Production, Land Surface Phenology and Evapotranspiration.

This presentation will focus on the current status of GBOV products and highlight recent developments and evolutions.

How to cite: Lerebourg, C., Grousset, R., Nativel, S., Carrière, J.-S., Clerici, M., Gobron, N., Muller, J.-P., Song, R., Dash, J., Paramanik, S., James, F., Ghent, D., Anand, J., Shukla, R., and Perez-Hoyos, A.: Copernicus Ground-Based Observations for Validation service (GBOV): overview and latest updates for EO data Cal/Val, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21819, https://doi.org/10.5194/egusphere-egu26-21819, 2026.

Understanding groundwater dynamics in arid environments is challenging due to sparse monitoring networks and strong anthropogenic influences. This study explores the potential of time-lapse microgravity observations to characterize shallow aquifer storage variability in Al-Ain City, United Arab Emirates. Repeated microgravity measurements were conducted at four monitoring wells over a one-year period between 2018 and 2019, alongside continuous groundwater-level observations, to investigate temporal changes in subsurface water mass. Observed gravity variations exhibit pronounced spatial and temporal contrasts across the study area, reflecting heterogeneity in aquifer response. Groundwater-level fluctuations over the monitoring period indicate notable seasonal and inter-annual variability, which is consistently mirrored in the gravity signal. By jointly analyzing gravity anomalies and water-level changes, variations in groundwater storage were quantified under a range of plausible specific yield values representative of shallow arid aquifers. Estimated storage changes indicate substantial redistribution of groundwater mass over the monitoring period, with corresponding volumetric changes on the order of several tenths to more than one million cubic meters, depending on local aquifer properties. The results demonstrate that microgravity monitoring provides an independent and spatially sensitive means of assessing groundwater storage dynamics, particularly in settings where conventional piezometric coverage is limited. This approach offers valuable insights into aquifer behavior under arid climatic conditions and highlights the broader potential of gravity-based methods for groundwater assessment, resource management, and hydrological characterization in data-scarce regions.

How to cite: Darwish, S.: Tracking Shallow Aquifer Storage Variability Using Time-Lapse Microgravity Measurements in an Arid Environment: Evidence from Al-Ain, UAE, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22102, https://doi.org/10.5194/egusphere-egu26-22102, 2026.

The University ‘G. d’Annunzio’ of Chieti Pescara Atmospheric Observatory (Ud’A Trabocchi) aims to investigate atmospheric chemistry, greenhouse gases evolution, atmosphere-soil exchanges and marine meteorology within a rural-marine setting. The facility has a 15 m tall tower with seven sample points: each every every 2 m. State-of-the-art instrumentation for long-term continuous measurements of CO2, CH4, N2O and isotopic ratio of CH4 and CO2 (Picarro); O3, NO, NO2, NOx, CO and SO2 (Thermo); NO2 (CAPS, Teledyne); CO2 flux (LI-COR); Radon (Mi.lan); Aerosol concentration and size distribution (SMPS, TSI); column observation of O3, NO2, SO2, HCHO (PANDORA 2S), Aerosol optical depth (CIMEL); GNSS reciver (Geoguard and Stonex); Meteorological station (Vaisala); Celiometer (Vaisala CL61). Finally, the station includes a UAV system equipped with meteorological sensors and low-cost sensor to detect CO2, CH4, O3 and NOxData of the first period of observation will be shown and will be discussed possible opportunity of collaborations and synergic activities.

How to cite: Di Carlo, P., Aruffo, E., Mascitelli, A., and Chiacchiaretta, P.: The University ‘G. d’Annunzio’ of Chieti Pescara Atmospheric Observatory (Ud’A Trabocchi): a new supersite for atmospheric observation and research in central Adriatic coast, Italy., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22380, https://doi.org/10.5194/egusphere-egu26-22380, 2026.

Meteorological calls on the mesoscale often hinge on change detection such as towering cumulus building, a gap opening for solar energy, or the first smoke plume rising under a convective cell. One of the most cost-effective datasets for detection of these phenomena is real-time, on-site imagery. The meteorological community has built remarkable capability with reliable, trustworthy surface/PBL observations spanning decades, and some network owners have recently begun to include webcam imagery at their sites as well, discovering many tangible benefits. However, for full situational awareness at a given location, the best imaging device is one that can capture the sky in all directions seamlessly.

This talk will introduce the WxStation, a new all-sky observing system currently undergoing extensive field testing within academic projects. The device combines professional grade in‑situ sensors with a 180° all‑sky camera to improve situational awareness. The addition of all-sky imagery into meteorological workflows can raise the effective resolution of mesoscale monitoring, particularly for cloud‑driven variability that impacts nowcasting, convective initiation, solar ramps, aviation ceiling/visibility, and wildfire situational awareness. A short image sequence quickly conveys a wealth of information to a trained observer—often faster and more intuitively than numbers alone can—making on-site imagery a powerful complement to conventional variables.

Furthermore, low‑power inference compute within the WxStation can automatically derive real‑time meteorological products (e.g., cloud fraction/type/motion) for assimilation into NWP and for wider analysis/climatological studies. In the long-term, these devices could provide insights equivalent to that of having a trained meteorological observer at every site 24/7/365. Two factors influence this outcome: (1) the deployment of enough devices to collect large datasets of high-quality imagery for labelling and (2) the development of AI interpretation models that are more capable per watt of compute power, specifically for meteorological tasks.

Prototype WxStation devices have been installed in real-world environments, including examples that will be highlighted during the talk. A deployment during the TEAMx intensive observing period (~3 summer months) in the European Alps captured frequent thunderstorms and rapid cloud‑field transitions. Another unit at the University of Leeds Farm (UK) has demonstrated day‑to‑day reliability in an agricultural setting. Some cold-weather testing down to –50 ºC will also be discussed. These deployments informed enclosure hardening, uptime targets, remote management, and early data intercomparisons against co‑located reference instruments.

The goals of this talk are to both engage and collaborate with the ground-based monitoring network community to propel this idea forward into new climates. Ideally, we seek network operators, research observatories, boundary‑layer testbeds, and emergency management–oriented networks to co‑design pilot evaluations in 2026. Pilots would quantify installation/ops burden (PoE power, mounting, maintenance), data pathways and latency, and product skill (cloud fraction/type/motion) versus co‑located references (e.g., ceilometers, trained observers). The aim is publishable evaluation results, a reusable ingest/QA template, and a clear path to broader operational use; including, if possible, exploratory NWP assimilation experiments (OSEs) as a stretch goal.

How to cite: Pickering, B.: Intelligent All-sky Cameras for Dense Mesoscale Observations: From Field Trials to Operational Pilots, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22806, https://doi.org/10.5194/egusphere-egu26-22806, 2026.

Small watersheds play a crucial role in sustaining river hydrology, ecological flows and local water security. However, they are increasingly threatened by climate change, rapid transformations of land use and escalation of anthropogenic pressures. These problems are worse in areas with little data, where few hydrological observations, sparse monitoring networks, and inconsistent long-term datasets make it hard to accurately assess vulnerability and make plans. To address this critical gap, this study introduces a unique and data-efficient Criteria Importance Through Intercriteria Correlation- Group Method of Data Handling (CRITIC-GMDH) hybrid framework, specifically developed to accurately assess watershed vulnerability in regions where large, continuous, or high-resolution datasets are unavailable. This interpretable decision-support approach integrates CRITIC for objective indicator weighting with the nonlinear modelling capability of the GMDH, enabling robust vulnerability prediction under constrained data conditions, overcoming key limitations of conventional hydrological models and black-box machine learning techniques. The framework incorporates eleven hydro-meteorological, geomorphological, and socio-economic parameters, including rainfall, temperature, runoff, watershed area, watershed length, water quality index, average slope, forest area, impervious area, population density, and highest flood level. The approach is demonstrated across four major river basins in Northeast India, such as Gomati, Haora, Khowai, and Manu, which represent highly sensitive and partially transboundary catchments. Future climate projections from CMIP6 SSP1-2.6 and SSP5-8.5 scenarios were used to compute the Vulnerability Index across decadal periods (2005–2065). Results show a significant escalation in vulnerability, particularly under SSP5-8.5, with Haora and Gomati exhibiting Vulnerability Index > 0.85, indicating extreme exposure to climate extremes, and urbanization stress. Sensitivity analysis identifies rainfall, runoff, and temperature as dominant controlling parameters, and validation through the Falkenmark indicator and green-blue water stress indices confirms emerging scarcity risks. The study provides a scientifically grounded pathway for watershed prioritization and climate-resilient planning, offering an adaptable methodological foundation for sustainable management of small river systems in data-scarce regions.

How to cite: Rudra Paul, A. and Kumar Roy, P.: Climate-Induced Vulnerability Assessment of Small Watersheds Using a CRITIC–GMDH Hybrid Model: A Methodology Tailored for Data-Scarce Regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4175, https://doi.org/10.5194/egusphere-egu26-4175, 2026.

Urban roads in fast-growing cities fall apart quickly, and everyone feels the impact—traffic slows down, accidents happen, and the city’s economy takes a hit. The old way of checking roads—sending people out to inspect them on foot—just doesn’t cut it anymore. It’s slow, expensive, and puts workers in harm’s way. So, we’ve built something better: an automated system that uses drones and AI to keep an eye on road conditions.

Here’s how it works. Drones fly over city streets, snapping high-resolution images that pick up everything from big potholes to tiny cracks. We run these images through our analytics pipeline. First, we use classic machine learning to weed out the stretches of road that are still in good shape. That way, the system doesn’t waste time on areas that don’t need attention.

Next, we use a deep learning model—based on YOLO, which stands for “You Only Look Once”—to hunt down and label the actual problem spots. We’ve trained this model using annotated drone photos, so it can handle tricky lighting or weird road surfaces. The model doesn’t just spot the defects—it also nails down where they are, how big they’ve gotten, and how bad the damage is.

But spotting problems isn’t enough. City agencies need to see this info and act on it, fast. So, we’ve built a web portal using OpenLayers and PostGIS that maps out every defect. Maintenance crews can sort issues by type or severity, pull up interactive maps, and even generate reports to plan repairs.

This whole setup is practical, affordable, and scales up easily for any city that wants to take road maintenance seriously. By bringing together drones, AI, and smart mapping, we’re giving city managers the real-time, reliable data they need to keep roads safe and traffic moving. And honestly, this system can help any city make smarter decisions about their roads and urban development.

How to cite: Manu, H. and Bhoopathi, S.: UAV-Based Road Defect Detection Using Hybrid Machine Learning Approach with Web GIS Visualization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6705, https://doi.org/10.5194/egusphere-egu26-6705, 2026.

EGU26-10741 | ECS | Orals | GI2.4

Machine Learning-Based Root-Zone Soil Moisture Estimation Using Satellite-Derived Surface Soil Moisture 

siddaling Bakka and Sudardeva Narayanan

Root-zone Soil Moisture (RZSM; 10–102 cm) is a critical variable for land–atmosphere interactions, plant water availability, groundwater recharge, and hydrological extremes; however, its reliable estimation at deeper layers over large spatial scales remains challenging. Ground-based monitoring networks such as the International Soil Moisture Network (ISMN) provide accurate multi-depth soil moisture observations, but their utility is constrained by sparse station distribution, high installation and maintenance costs, and limited spatial coverage (Dorigo et al. 2011). In contrast, microwave remote sensing based satellite missions, including Soil Moisture Active Passive (SMAP), Soil Moisture and Ocean Salinity (SMOS), and Sentinel-1, offer frequent and spatially continuous SM observations but are sensitive only to near-surface conditions (top ~5 cm), leaving deeper soil layers unobserved. This disparity between depth-limited in-situ observations and surface-focused satellite measurements motivates the present study to develop a machine learning based framework to estimate RZSM from satellite-derived surface SM by incorporating temporal memory and forcing. This approach effectively captures persistence effects and vertical moisture transfer, which are essential for accurate prediction of deeper SM layers (Pal &Maity, 2019). Multi-depth SM observations from 5 to 102 cm, obtained from ISMN stations and categorized according to USDA Hydrologic Soil Groups (HSG A–D; four stations per HSG), account for differences in soil water movement and retention behaviour (Ross et al. 2018). For each soil group, Support Vector Regression (SVR) and Random Forest (RF) models were trained using a sequential, depth-wise prediction strategy comprising four depth transitions: 5–10 cm, 10–20 cm, 20–51 cm, and 51–102 cm. Model evaluation demonstrates strong predictive performance across all depth intervals (R² = 0.85–0.95 for RF and 0.63–0.95 for SVR at validation sites), indicating that HSG classification effectively captures soil-specific SM dynamics. The trained models successfully generate comprehensive RZSM profiles using satellite-derived SM from the SMAP mission.These profiles are rigorously validated against ground-based observations and demonstrate strong applicability across diverse landscapes lacking direct subsurface measurements.

How to cite: Bakka, S. and Narayanan, S.: Machine Learning-Based Root-Zone Soil Moisture Estimation Using Satellite-Derived Surface Soil Moisture, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10741, https://doi.org/10.5194/egusphere-egu26-10741, 2026.

EGU26-11280 | Orals | GI2.4

Combining different hydraulic methods to estimate the discharge from Combined Sewer Overflows (CSO) into streams. 

Michael Robdrup Rasmussen, Mathias Ulsted Jackerott, Janni Mosekær Nielsen, Ida Kemppinen Vestergaard, and Jesper Ellerbæk Nielsen

Combined Sewer Overflows (CSOs) in cities can play a significant role in the morphology and hydraulic performance of streams near urban areas. A complete urban drainage system is often modelled by a dedicated hydrological/hydraulic model (e.g., SWMM or Mike+). However, these models must be calibrated against observations. Especially the flow from CSOs is difficult to estimate. The quality of the data and the drainage models depend on the accuracy of the overall mass balance of the drainage system. If it is not possible to estimate the discharge from, for example, a CSO, the results from other parts of the system become unreliable.

This research evaluates flow dynamics through a multi-methodological approach where the CSO is evaluated by theoretical models, CFD models, experimental work in a laboratory, and a new innovative method where the noise from a CSO is analyzed. The sound is both analyzed directly and by training a machine learning model on the laboratory experiments. The result is a hybrid model filtering all the estimates to one flow estimate. CFD has been used to model the specific CSO to take a Q-h relationship into account, and to generate a so-called catalog method. In this method, multiple variations of geometry are simulated in a free-surface CFD model to cover many different geometries, and general equations are extracted from these simulations.

The hybrid approach opens the door to a new way of estimating interactions between the urban water cycle and the receiving waters. Applying edge processing makes it possible to continuously adapt to local conditions that were not present during the calibration and validation of the model. Edge processing involves signal processing and modeling at the measuring point, where the maximum bandwidth of the sensor data is available and can be used for the most accurate data estimation.

How to cite: Rasmussen, M. R., Jackerott, M. U., Nielsen, J. M., Vestergaard, I. K., and Nielsen, J. E.: Combining different hydraulic methods to estimate the discharge from Combined Sewer Overflows (CSO) into streams., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11280, https://doi.org/10.5194/egusphere-egu26-11280, 2026.

EGU26-12001 | Orals | GI2.4

Evaluating Climate Change Impacts and Adaptation Options for Paddy Yield Using Data-Curated Modelling in Goa, India 

Ankit Balvanshi, Jayakumar Kv, and Venkappayya r Desai

This study investigates the coastal-region impacts of climate change on rice yield in Goa, India, a monsoon-driven agroecosystem highly dependent on paddy cultivation and vulnerable to rainfall variability, salinity intrusion, and rising temperatures. The study aims to (i) estimate future crop evapotranspiration (ETc) and rice yield projections under different Shared Socioeconomic Pathways (SSP 2.6, SSP 4.5, and SSP 8.5), and (ii) assess the effectiveness of adjusting planting dates, along with the integration of drought-resilient cultivars, alternate wetting and drying (AWD) irrigation, and soil management practices, as adaptation strategies to mitigate yield reductions. To achieve these objectives, the CropWat and AquaCrop models were employed, using statistically downscaled CMIP6 CESM2 climate data.

The AquaCrop model was calibrated using data from 1994 to 2004 and validated for the period 2005–2014, demonstrating strong performance metrics (Nash–Sutcliffe Efficiency = 0.86, RMSE = 278.5, r² = 0.93). Our findings indicate that projected climatic changes pose a significant threat to rice yield stability in the region. Rising temperatures and shifting monsoon patterns are expected to elevate evapotranspiration demand by 10–14%, thereby intensifying irrigation requirements even in high-rainfall areas.

In response, adjusting planting dates emerged as a promising adaptation strategy. Specifically, delaying planting by 5 days until 2070 and by 10 days from 2071 to 2099 significantly mitigated yield declines across all SSP scenarios. An optimum 10-day delay in planting was found to recover up to 17% of yield losses under SSP 2.6 and SSP 4.5. Furthermore, compound strategies—including drought-tolerant rice cultivars, AWD irrigation, and improved soil management—provided up to 25% additional yield gains. These integrated approaches not only improved crop water productivity but also stabilized yields under moderate emission pathways. However, under the high-emission SSP 8.5 scenario, yield reductions remained substantial (up to 20%) due to increased temperature stress and shortened grain-filling duration, underscoring the limits of adaptation under extreme climate conditions.

The results highlight the importance of temporally optimized sowing schedules, integrated irrigation management, and improved soil practices for enhancing the resilience of coastal rice systems. This study further demonstrates that reliable data curation, model calibration, and parameter selection are essential to improving predictive accuracy in agro-hydrologic modelling. The findings emphasize the need for consistent methodological frameworks that couple climate projections with process-based crop models to assess adaptation effectiveness under uncertain future conditions.

Overall, the study provides actionable insights for strengthening the accuracy and reliability of water- and climate-based agricultural modelling frameworks. The outcomes contribute to developing climate-resilient strategies for paddy cultivation in coastal India, reinforcing the broader understanding of model validation, uncertainty reduction, and data-driven adaptation in hydrologic and agricultural research.

How to cite: Balvanshi, A., Kv, J., and Desai, V. R.: Evaluating Climate Change Impacts and Adaptation Options for Paddy Yield Using Data-Curated Modelling in Goa, India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12001, https://doi.org/10.5194/egusphere-egu26-12001, 2026.

EGU26-12042 | ECS | Posters on site | GI2.4

Strategies for spatial leave-one-out cross-validation 

Cristina Olimpia Chavez Chong, Cécile Hardouin, and Ana Karina Fermin Rodriguez

The purpose of the talk is to discuss spatially adapted cross-validation methods that maintain sufficient separation between training and validation sets, thus providing more accurate estimates of model risk. We begin by reviewing various spatial cross-validation techniques, including spatial blocked cross-validation and spatial leave-one-out, under scenarios of low to strong spatial dependence. We then propose a practical framework for determining an optimal “buffer size” for spatial leave-one-out that reduces autocorrelation between training and validation subsets. This framework is further enhanced by a parametric bootstrap approach designed to approximate the true risk in single-realization settings. Simulation experiments confirm that these methods effectively capture the underlying spatial structure, leading to more reliable risk estimation.

How to cite: Chavez Chong, C. O., Hardouin, C., and Fermin Rodriguez, A. K.: Strategies for spatial leave-one-out cross-validation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12042, https://doi.org/10.5194/egusphere-egu26-12042, 2026.

EGU26-13261 | ECS | Orals | GI2.4

Flow Modulation and Wave Impact Reduction by Retreated Crown Walls in Vertical Breakwaters 

Shaik Firoj and Mohammad Saud Afzal

This study investigates wave-induced flow behaviour around vertical breakwaters with retreated crown wall using numerical simulations. Previous experimental work has shown that moving the crown wall landward can reduce wave forces, moments, and overtopping. However, the associated flow mechanisms near the wall and trunk region have not been examined in detail. In this work, the open-source CFD model REEF3D is used to simulate regular wave interaction for crown wall retreat configuration. The model solves the Reynolds-averaged Navier–Stokes equations, with a level set method for free-surface tracking and a k–ω turbulence closure. The numerical results are first validated against published experimental data to ensure accuracy. The simulations provide detailed information on velocity fields, vortex formation, and flow separation during wave impact and overtopping. The results show that retreating the crown wall modifies the local flow structure, leading to a redistribution of momentum and a reduction in direct wave impact on the wall. These findings help to clarify the hydrodynamic role of retreated crown wall in vertical breakwater design.

How to cite: Firoj, S. and Afzal, M. S.: Flow Modulation and Wave Impact Reduction by Retreated Crown Walls in Vertical Breakwaters, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13261, https://doi.org/10.5194/egusphere-egu26-13261, 2026.

Watershed hydrodynamics is governed by various hydrological flow processes that occur at different spatiotemporal scales. Most hydrological models couple the surface flow solver with the standard empirical infiltration models for flood propagation modeling. However, the empirical infiltration models are not applicable for heterogeneous and anisotropic soils and shallow groundwater tables, which are most vulnerable to waterlogging problems. Hence, simultaneous and integrated modeling of the surface and subsurface flow processes is essential for the continuous monitoring of watershed hydrodynamics. A physically based unified multi-region, multi-process watershed model integrates the various hydrological flow components in different regions through unique coupling mechanisms at the interfaces. The current work presents a Finite Volume (FV) method-based watershed flow model developed using the OpenFOAM® framework [1]. The developed model framework utilizes the ‘multi-region’ structure from the OpenFOAM® library to integrate the OpenFOAM®-based solvers for the individual processes of surface overland flow [2,3] and saturated-unsaturated subsurface flow [4] through the imposition of appropriate interface boundary conditions or addition of source/sink terms at the interfaces of the flow regions. The surface flow component is modeled using the diffusive wave or the zero-inertia (ZI) approximation of the two-dimensional (2D) depth-averaged shallow water equations (SWE). On the other hand, the flow through the variably saturated subsurface media is modeled using the ‘mixed form’ of the 3D modified Richards Equation. The flux exchange between the surface and subsurface regions (infiltration or exfiltration rate) is modeled using a switching algorithm to impose the boundary condition on the interface between the two regions. The algorithm changes the interface to a Dirichlet or a Neumann type boundary condition based on the rainfall intensity and the saturated hydraulic conductivity of the ground surface. A stabilized and adaptive time-stepping algorithm has been implemented to ensure smooth convergence of the iterative technique used for linearizing the nonlinear governing equations. The developed model is equipped with parallelization strategies to be run on multi-core processors, which is essential for increased computational efficiency while solving regional-scale watershed flow problems. The developed watershed model has been verified and validated against the standard benchmark problems on saturation excess and infiltration excess from the literature. Moreover, the applicability of the developed model has been extended to solve complex hydrological problems on exfiltration occurring over natural catchments, yielding satisfactory results.

References

[1] Jasak, H., A. Jemcov, Z. Tukovic. (2007). OpenFOAM: A C++ library for complex physics simulations. In Vol. 1000 of Proc., Int. Workshop on Coupled Methods in Numerical Dynamics,1–20. Dubrovnik, Croatia: Inter-University Center

[2] Dey, S., Dhar, A. (2024). Applicability of Zero-Inertia Approximation for Overland Flow Using a Generalized Mass-Conservative Implicit Finite Volume Framework. Journal of Hydrologic Engineering, 29(1), 04023042.

[3] Dey, S. (2025). zeroInertiaFlowFOAM – a OpenFOAM®-based computationally efficient, mass-conservative, implicit zero-inertia flow model for flood inundation problems on collocated grid-systems (No. EGU25-17402). Copernicus Meetings.

[4] Dey, S., & Dhar, A. (2022). Generalized mass-conservative finite volume framework for unified saturated–unsaturated subsurface flow. Journal of Hydrology, 605, 127309.

How to cite: Dey, S. and Dhar, A.: An OpenFOAM®-based coupled surface-subsurface flow model for simulating watershed hydrodynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13540, https://doi.org/10.5194/egusphere-egu26-13540, 2026.

EGU26-16374 | ECS | Orals | GI2.4 | Highlight

Reorganization of Heatwave Day Regimes across India under Recent and Near Future Warming 

Srikanth Bhoopathi and Manali Pal

Heatwaves are among the most rapidly intensifying climate extremes over India, yet their evolving spatial characteristics under recent and near future climate change remain inadequately quantified. This study examines the spatio-temporal variability of Heatwave Days (HWDs) across India using daily maximum temperature from the India Meteorological Department (IMD) gridded dataset for the historical period 1975-2024 and extends the analysis to the near future (2025-2044) using CMIP6 climate projections. Heatwave days are identified at each grid point using a calendar day based percentile approach, where daily maximum temperature exceeding the local 95th percentile threshold for the same calendar day, computed over a fixed reference period of 1981-2010, is classified as a heatwave day. Grid wise cumulative and decadal HWDs are analysed to assess long-term exposure and spatial redistribution. To objectively identify dominant heatwave regimes, Self-Organizing Maps (SOMs) are employed using multiple HWD metrics, enabling classification of regions with distinct heatwave characteristics and temporal evolution. Observational results indicate a clear reorganization of heatwave patterns over India. During the late 20th century (1975-1994), HWD accumulation is largely limited to north-western and parts of central India, typically ranging between 26 to 50 days per decade, with most eastern and peninsular regions experiencing fewer than 25 HWDs. From the mid-1990s onward, a pronounced intensification and spatial expansion is evident. By 2005-2014, large parts of central and eastern India exhibit decadal HWDs in the range of 51 to 100 days. The most recent decade (2015-2024) shows widespread moderate to high HWDs accumulation across the country, with several regions of central, eastern, and peninsular India experiencing 101 to 150 HWDs, and localized hotspots exceeding 150 days per decade. Future HWDs for 2025-2044 are derived from daily maximum temperature projections of the MPI-ESM1-2-HR model under the SSP2-4.5 scenario. The near-future decadal projections (2025-2034 and 2035-2044) indicate a continued intensification and spatial expansion of HWDs, with extensive areas of north-western, central, and peninsular India experiencing 151 to 250 HWDs per decade, and emerging hotspots exceeding 250 to 350 days, particularly over parts of north-western and southern India. Eastern India also shows a marked transition toward higher HWDs classes, indicating increasing regional vulnerability. Overall, the combined observational and CMIP6 based analysis demonstrates a transition toward widespread and persistent heatwave exposure across India in both recent decades and the near future. The integration of a grid specific, calendar day based percentile definition with SOM based classification provides a robust framework for identifying evolving heatwave regimes and supports improved heat risk assessment, climate adaptation planning, and early warning strategies under continued warming.

How to cite: Bhoopathi, S. and Pal, M.: Reorganization of Heatwave Day Regimes across India under Recent and Near Future Warming, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16374, https://doi.org/10.5194/egusphere-egu26-16374, 2026.

Considering the dearth of gauge-based rainfall observations at desirable resolution, it becomes immensely challenging to quantify and monitor droughts, especially over the developing countries. This can be circumvented by utilizing the high-resolution open-access rainfall products. This study is envisaged with the objective to assess the spatiotemporal variation of meteorological droughts over the Bundelkhand region, India. The multi-source weighted-ensemble precipitation (MSWEP), a blended product of global gauge-based, satellite-based and reanalysis precipitation datasets, is utilized for a period of 44 years (1980-2023). The MSWEP rainfall is bias-corrected with respect to the India Meteorological Department (IMD) gridded observation dataset for the 14 districts in the region. Using the corrected rainfall product, the droughts over each district are characterized by Standardized Precipitation Index (SPI) at three different timescales, i.e., the SPI-3, SPI-6 and SPI-12 are used to model short-term, intermediate-term and long-term droughts, respectively. A drought severity index (DSI) is proposed considering the probability of droughts in different severity classes (i.e., near-normal, moderate, severe and extreme). Further, the trend analysis of SPI at different timescales is carried out using Modified Mann-Kendall (MMK) test. The results reveal the MSWEP dataset’s problems in capturing higher quantiles, which affects the probabilistic distribution used for quantifying drought events. However, the bias-corrected MSWEP product showed an excellent match with the IMD gridded data, thereby substantiating its applicability over the Bundelkhand Region. The region is found to be prone to droughts with an increasing trend of dryness. The novel approach of DSI is found to distinguish the drought severity levels at district-scale, which can be helpful for planning and management of droughts. Overall, this study provides critical insights on the drought characterization using state-of-the-art datasets and innovative approaches, which can also be extended to other drought-prone regions of the world.

 

Keywords: Bias-correction; Bundelkhand; DSI; MSWEP; MMK; SPI

How to cite: Swain, Dr. S.: A statistical approach of mapping drought severity using bias-corrected blended dataset over a semi-arid region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18814, https://doi.org/10.5194/egusphere-egu26-18814, 2026.

EGU26-18906 | Orals | GI2.4

Passive Acoustic Characterization of Marine Bedload Transport Based on Interparticle Collision Dynamics 

Debasish Dutta, Armelle Jarno, Hugues Besnard, Bruno Morvan, and Francois Marin

Marine sediments are very important for keeping the coast stable and protecting the shoreline naturally. However, anthropogenic activities can greatly change how sediment moves, making their accurate monitoring essential. In marine settings, understanding bedload sediment transport can be challenging due to conventional methods reliant on visual observations or direct sediment sampling tend to be intrusive, spatially constrained, and inadequate for long-term or continuous monitoring. In this situation, passive underwater acoustics is a promising non-intrusive option that can provide continuous monitoring with high temporal resolution. This study investigates the acoustic signatures related to marine bedload transport, focusing particularly on the sounds generated by interparticle collisions of mobile sediments. A series of controlled laboratory experiments are performed utilising simplified experimental arrangements in which artificial sediments (spherical glass beads) are mobilised under oscillatory motion that simulates wave-induced seabed forcing. We use glass beads of different sizes to create idealised bedload conditions, and we use an oscillating plate to control the movement of the particles. Hydrophones placed close to the sediment bed record acoustic pressure signals. The recorded acoustic signals are analyzed in both the time and frequency domains. Individual particle impacts are characterised by short transient acoustic events, and spectral analyses show clear peak frequencies that are linked to sediment motion. The results indicate that the peak frequency of the acoustic spectrum is predominantly determined by particle diameter and is additionally influenced by the amplitude and frequency of the applied oscillatory motion. These observations align with theoretical models, such as those suggested by Thorne (1985), that explain the generation of pressure waves during underwater particle collisions. To further explore the mechanisms of sound generation, experiments are conducted with both smooth and rough beds below the beads layers. The analysis reveals the existence of sediment-specific acoustic signatures, facilitating the differentiation of particle sizes according to their spectral characteristics. This study illustrates the significant potential of passive acoustic methods for the remote monitoring of marine bedload transport. The study offers novel insights into sound generation mechanisms linked to sediment motion across various particle sizes, motion amplitudes, and bed configurations, utilising a combination of laboratory experiments, theoretical frameworks, and comprehensive spectral analysis, with direct implications for intricate coastal and offshore environments.

How to cite: Dutta, D., Jarno, A., Besnard, H., Morvan, B., and Marin, F.: Passive Acoustic Characterization of Marine Bedload Transport Based on Interparticle Collision Dynamics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18906, https://doi.org/10.5194/egusphere-egu26-18906, 2026.

Wildfires in radioactively contaminated regions, such as the Chernobyl Exclusion Zone, pose a growing environmental threat by resuspending long-lived radionuclides into the atmosphere. However, accurately quantifying the redistribution of these radionuclides remains challenging. Existing top-down inversion studies often oversimplify source terms by assuming fixed particle sizes and release altitudes, which hinders the precise evaluation of transport mechanisms and deposition footprints.

To address this gap, this study proposes a novel multi-component source term inversion framework to simultaneously reconstruct the time-varying release profiles of 137Cs across multiple particle sizes (0.4, 8, and 16 μm) and seven vertical layers (0-3000 m). We improved the Projected Alternating Minimization with L1-norm and Total variation regularization (PAMILT) algorithm by incorporating a TV-regularized initialization and a Bayesian optimization scheme for hyperparameter tuning to ensure robust convergence. These retrieved source terms were then coupled with the WRF-Chem model using size-resolved microphysics to conduct a high-resolution simulation of the April 2020 Chernobyl wildfires.

Validation results demonstrated exceptional agreement between the simulated and observed concentrations, achieving a Pearson correlation coefficient of 0.996 and reducing maximum relative biases from over 106 to generally below 102. The inversion estimates a total 137Cs release of approximately 836 GBq. This release was dominated by fine particles (0.4 μm, ~54%) and low-altitude injections, with 58.1% occurring below 1 km. Crucially, our WRF-CHEM simulations reveal a decoupling between emission abundance and deposition impact. Although fine particles dominate the source term, coarse particles (16 μm) control the near-field deposition flux due to rapid gravitational settling. These coarse particles exhibit a "transport plateau" beyond roughly 800 km, whereas fine particles show a linear growth in transport distance constrained only by meteorological dispersion. Furthermore, we identified distinct deposition signatures. Dry deposition manifests as a continuous spatial accumulation or "creeping" effect. In contrast, wet deposition drives "step-wise" long-range transport, triggering sudden and pulse-like removal events far from the source.

These findings provide critical insights into the complex mechanics of radionuclide redistribution and offer a refined methodology for assessing the environmental impact of future wildfire events in contaminated zones.

How to cite: Xu, Y. and Fang, S.: Unraveling size-resolved 137Cs resuspension and deposition from the 2020 Chernobyl Wildfires via multi-component inversion and WRF-Chem simulation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2436, https://doi.org/10.5194/egusphere-egu26-2436, 2026.

The discharge of ALPS-treated water from the Fukushima Daiichi Nuclear Power Plant (FDNPP) in August 2023 renewed concerns regarding radionuclide dispersion in the North Pacific, particularly in the waters surrounding Taiwan. This event highlighted the need to assess not only releases from Fukushima but also the cumulative influence of multiple nuclear power plants operating within the region. To investigate potential dispersion patterns under simultaneous multi-source discharges, this study employed a particle tracking model coupled with the Semi-implicit Cross-scale Hydroscience Integrated System Model (SCHISM), together with a two-dimensional Gaussian diffusion model, to simulate tritium dispersion in surface seawater from six facilities located in the western North Pacific region during 2023–2024: FDNPP, Wolsong, Qinshan, Fuqing, Daya Bay, and the Maanshan Nuclear Power Plant (NPP3 in Taiwan). Also, the modeled tritium concentrations in the Pacific area were compared with background seawater levels reported in the IAEA Marine Radioactivity Information System (MARIS) database. This comparison provided a baseline consistency check to examine whether the simulated tritium distributions were influenced by large-scale ocean circulation and cumulative multi-source discharges.

To further evaluate potential local impacts around Taiwan, seven representative monitoring sites were selected to capture spatial variability across different coastal sectors and offshore regions, including Kinmen, Matsu, the Tamsui River Estuary, Cijin, the Zhuoshui River Estuary, Guishan Island, and FRI-ST-15 (a Fisheries Research Institute monitoring station). These sites were used to examine seasonal concentration responses associated with eastern, western, northern, and southern waters, as well as offshore island environments. The results indicate that tritium released from multiple sources was transported northward by the Kuroshio Current, reaching southern Japan and extending eastward to approximately 180°E. In the northwestern waters of Taiwan, including Kinmen and Matsu, contributions from Fuqing and Qinshan were dominant. At Kinmen, Fuqing’s contribution reached maximum values immediately after discharge and remained significant into early spring, whereas the contribution from Qinshan was comparatively smaller. At Matsu, Qinshan’s contribution increased approximately one month after discharge, decreased by late winter, and reached a secondary maximum in the subsequent winter, while Fuqing’s contribution increased during late winter and maintained a moderate influence thereafter.

Finally, some sensitivity analyses assuming a 50-fold increase in discharge concentrations were conducted to assess potential variability and relative influence among sources. The results indicated negligible influence from Wolsong and FDNPP, whereas discharges from Qinshan, Fuqing, Daya Bay, and NPP3 produced more pronounced, seasonally modulated signals that diminished with increasing distance from Taiwan.

How to cite: Chiang, Y. and Huang, P.-C.: Modeling the Regional Dispersion of Continuous Multi-Source Tritiated Water Discharges in Surface Waters Around Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3203, https://doi.org/10.5194/egusphere-egu26-3203, 2026.

EGU26-3623 | ECS | Posters on site | GI2.5

Transport of Particulate ¹³⁷Cs in the Coastal Area off Fukushima Based on Long-Term Continuous Measurement 

Shun Satoh, Kazuya Yoshimura, Toshiharu Misonou, and Daisuke Tsumune

Since the accident at the Fukushima Daiichi Nuclear Power Station in March 2011, numerous studies have examined the behavior of radioactive cesium (¹³⁷Cs) in the ocean. Recent studies suggest that large amounts of particulate ¹³⁷Cs deposited on land are transported to coastal waters via rivers, becoming a major source of coastal ¹³⁷Cs input. Although numerical simulations and conceptual studies indicate that particulate ¹³⁷Cs entering coastal waters can be transported offshore through sedimentation, resuspension, and lateral transport, long-term, high-frequency observational studies remain limited. In this study, we evaluated the transport of particulate ¹³⁷Cs in coastal area off Fukushima using one year of continuous measurement data from multiple moored systems.

Moored systems were deployed at three sites near the mouth of the Ukedo River, where current velocity, current direction, and turbidity were continuously measured from February 2017 to February 2018. These data were combined with regularly collected measurements of suspended solid concentrations (mg/L) and particulate ¹³⁷Cs concentrations (Bq/L) to estimate hourly lateral fluxes of particulate ¹³⁷Cs (Bq/h). The study area is influenced by ¹³⁷Cs inputs transported via the Ukedo River, and the relationships between particulate ¹³⁷Cs fluxes and seasonal variability, meteorological conditions (waves, precipitation, and wind), and river discharge were analyzed. Furthermore, by focusing on differences in fluxes among the observation sites, we examined the factors controlling riverine input and transport variability from the coastal area toward offshore.

This study uses long-term monitoring data off Fukushima to improve understanding of particulate ¹³⁷Cs transport processes in coastal waters and to provide observational constraints for future numerical modeling studies.

How to cite: Satoh, S., Yoshimura, K., Misonou, T., and Tsumune, D.: Transport of Particulate ¹³⁷Cs in the Coastal Area off Fukushima Based on Long-Term Continuous Measurement, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3623, https://doi.org/10.5194/egusphere-egu26-3623, 2026.

Since the commencement of the ALPS-treated water discharge from Fukushima Daiichi on 23 August 2023, an operational forecasting system developed in Taiwan has been established to provide daily seven-day predictions of tritium dispersion in the North Pacific. The system integrates the real-time CWA-OCM with particle tracking and grid-based concentration diffusion modules, driven by hourly discharge data reported by TEPCO. The computational domain covers the Kuroshio–Kuroshio Extension and adjacent marginal seas, with refined resolution near the outlet to capture dispersion within approximately 3 km. Validation against TEPCO tritium monitoring data at 12 sites across three representative batches (1, 2 and 12) demonstrated that the system successfully reproduced both the spatial distribution and temporal evolution of tritium concentrations, with modeled maxima typically within the observed range of 10–20 Bq/L. However, the model slightly underestimated the peak values, and simulated concentrations decreased more rapidly than observed during the five-day post-discharge period. This discrepancy is likely attributed to the absence of the jet effect in the current model. Therefore, we will continue to refine the model and integrate these improvements into our operational forecasting system.

How to cite: Zeng, H.-T., Teng, J.-H., and Chiang, Y.: Validation of the Refined Daily Forecasting System for ALPS Treated Water Dispersion Against Observation Data near the Fukushima Outlet, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4581, https://doi.org/10.5194/egusphere-egu26-4581, 2026.

EGU26-5031 | Posters on site | GI2.5

Assessment of the Kuroshio Large Meander’s Impact on the Dispersion Pathways of Fukushima Tritium-treated Water 

Yen-Ju Chu, Hui-Ting Zeng, Jen-Hsin Teng, and Chi-Hung Wang

The discharge of ALPS treated water from the Fukushima Daiichi Nuclear Power Station into the North Pacific Ocean has necessitated a detailed assessment of long-term dispersion pathways. The transport of this ALPS treated water is primarily governed by the Kuroshio Extension (KE) system. However, the upstream Kuroshio has been experiencing a persistent “Kuroshio Large Meander (KLM)” event since August 2017. Since the variability of the KE is dynamically linked to the path of the Kuroshio south of Japan, understanding how the KLM modulates the downstream flow field is critical for evaluating environmental impacts.

In this study, we investigate the influence of the KLM on the dispersion of tritium-treated water by Lagrangian particle tracking model with a continuous release scheme. The model was forced by ocean current data from the Hybrid Coordinate Ocean Model (HYCOM) to capture the spatiotemporal variability of the Kuroshio Current. We specifically examined the differences in transport patterns during the KLM period (2017–2022) versus non-meander period (2011–2016).

Preliminary results indicate that the presence of the upstream Large Meander induces specific downstream responses in the Kuroshio Extension that distinctively deviate from the reference non-meander period. We focus on how the KLM modulates the stability and position of the KE jet, thereby altering the initial advection pathways of the ALPS treated water. The analysis aims to clarify whether these KLM-induced changes in the KE system act to retard zonal transport or enhance regional retention, creating significant discrepancies in tracer arrival times and concentration fields between the two periods.

This study quantifies these deviations and discusses the implications of the “Kuroshio-Kuroshio Extension coupling” mechanism in determining the dispersion patterns and concentration distributions of passive tracers. The findings highlight the necessity of incorporating low-frequency climate variability into environmental risk assessments for oceanic discharges.

How to cite: Chu, Y.-J., Zeng, H.-T., Teng, J.-H., and Wang, C.-H.: Assessment of the Kuroshio Large Meander’s Impact on the Dispersion Pathways of Fukushima Tritium-treated Water, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5031, https://doi.org/10.5194/egusphere-egu26-5031, 2026.

Overview of the observation and simulation studies regarding radiocesium resuspension from contaminated land surfaces in Fukushima is presented based on our previous papers, Kajino et al., ACP (2016), Kajino et al., ACP (2022), Watanabe et al., ACP (2022). The long-term atmospheric behaviors of radiocesium have been understood based on the long-term measurements of concentration and deposition of radiocesium in Fukushima city (Watanabe et al., 2022) and numerical simulations considering radiocesium resuspension from soil and vegetation (Kajino et al., 2022). However, there is still one unresolved issue remains: exceptionally high monthly cumulative deposition amounts in January in Fukushima city even though the monthly atmospheric concentrations are not very large. We therefore hypothesized that the giant aerosol resuspension due to snow removal work or passing vehicles that carried radiocesium deposited in the vicinity of the observation site into the deposition sampler, but not into the air sampler, since the gravitational velocity of such giant aerosols is too high to collect by the air sampler. This additional source is referred to as secondary resuspension. The numerical assessment and field observations of the secondary resuspension will also be presented at the conference. 

How to cite: Kajino, M.: Resuspension of radiocesium from contaminated land surfaces in Fukushima: source contributions from soil, vegetation, and other sources, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8529, https://doi.org/10.5194/egusphere-egu26-8529, 2026.

EGU26-8971 | Posters on site | GI2.5

Four decades after Chornobyl: long-lived radionuclide legacy and sustainable land and resource use   

Yasunori Igarashi, Vasyl Yoschenko, Yuichi Onda, Valentyn Protsak, Gennady Laptev, Dmytrii Holiaka, Dmitry Samoilov, Serhii Kirieiev, Alexei Konoplev, and Jim Smith

Chornobyl remains the world’s longest-running field-scale experiment of how societies and ecosystems respond to persistent, spatially heterogeneous contamination. Yet sustainability-relevant synthesis across environmental compartments—soils, forests, surface waters, groundwater, and the evolving exposure landscape—remains fragmented, often separated into radiological, ecological, or regulatory discussions. Here we integrate four decades of observations in and around the Chornobyl Exclusion Zone to evaluate what has changed, what has not, and what this implies for sustainable land and resource use under long-lived hazards. We assess four compartment-linked insights: (isoils as the primary long-term reservoir of fallout: inventories of 137Cs and 90Sr have declined but remain highly heterogeneous, while vertical redistribution and particle-associated processes increasingly govern mobility and bioavailability; (ii) forests as both sink and pathway: radionuclides are continuously recycled through litter and biomass, and contrasting within-tree distributions of 137Cs versus 90Sr impose distinct constraints on wood utilization and circular-economy strategies; (iii) aquatic systems as delayed but persistent exporters: multi-decadal river records exhibit long tails and sensitivity to disturbances (e.g., floods, fires), while groundwater pathways—especially for 90Sr—represent enduring, often weakly observed legacy with clear management relevance; and (iv) exposure landscapes that evolve nonlinearly: spatiotemporal changes in dose fields complicate re-zoning decisions that depend on both scientific evidence and societal acceptance. We synthesize these findings into a sustainability framework that links environmental dynamics to governance choices, including conditional resource use, monitoring prioritization, and intergenerational risk trade-offs. These lessons generalize to other nuclear accidents and to broader classes of persistent contaminants where returning to baseline is unrealistic and sustainability must be designed under enduring constraints. 

How to cite: Igarashi, Y., Yoschenko, V., Onda, Y., Protsak, V., Laptev, G., Holiaka, D., Samoilov, D., Kirieiev, S., Konoplev, A., and Smith, J.: Four decades after Chornobyl: long-lived radionuclide legacy and sustainable land and resource use  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8971, https://doi.org/10.5194/egusphere-egu26-8971, 2026.

The Fukushima Daiichi Nuclear Power Plant (FDNPP) accident contaminated large areas of the Pacific Ocean with different radionuclides. However, not all areas are studied equally. For example, the Sea of Okhotsk is one of the least studied regions, with almost no measurement data available. In the current study, we applied the Lagrangian particle tracking model Parcels V3.0 to simulate the trajectories of virtual particles containing radionuclides in the Pacific Ocean. Here, the output from the KIOST-MOM circulation model is used. It includes monthly mean climatic data for 3D currents (U, V, W components of water velocity) and vertical diffusivity coefficients. Coefficients for horizontal diffusion are calculated using the Smagorinsky formula.

Virtual particles were emitted at the location of the FDNPP during 31 days (26 Mar to 25 Apr 2011), when 96.6% of the total amount of radionuclides was released directly to the ocean. Each particle initially contained a certain activity of radionuclides (137Cs, 134Cs, 90Sr, 3H, 129I) proportionally to the estimated total release of each radionuclide. The activity of each radionuclide inside the particle decreased according to radioactive decay with the corresponding half-life. The atmospheric deposition of radionuclides on the sea surface was not considered here.

Model results were validated on the 134Cs concentrations in the Northeastern Pacific in areas with measurement data after 2012, when the impact of atmospheric deposition decreased. For the Sea of Okhotsk, the concentrations of 5 radionuclides were calculated and analyzed. For particles that reached the Sea of Okhotsk, we calculated statistical characteristics based on Lagrangian trajectories: visitation frequency, mean age, and representative trajectory, which demonstrated the pathways of water masses transporting radioactivity from FDNPP to the Sea of Okhotsk.

How to cite: Bezhenar, R., Tateda, Y., Inomata, Y., Kim, K. O., and Kim, H.: Lagrangian trajectories of Fukushima Daiichi NPP originated water, transported by large-scale circulation in the North Pacific Ocean, and reached the Sea of Okhotsk, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9903, https://doi.org/10.5194/egusphere-egu26-9903, 2026.

Validating the reproducibility of ocean dispersion models used in prior environmental impact assessments of ALPS-treated water release is essential for evaluating their applicability. In this study, we conducted reproduction simulations using actual release records together with observed meteorological and oceanographic conditions, and quantitatively compared the results with seawater monitoring data.

Model results were compared with tritium monitoring data collected by TEPCO, the Ministry of the Environment, the Nuclear Regulation Authority, and Fukushima Prefecture. The release was assumed to instantaneously disperse within a model grid (147 m × 186 m), with release scenarios prescribed for both the surface layer and the near-bottom layer at a depth of 10 m. As the actual discharged water is expected to rise upward from the seabed, results from the surface-release simulation are mainly discussed. Geometric means were used for model–observation comparisons to reduce the influence of outliers. Since background tritium concentration is not explicitly represented in the model, a constant background of 100 Bq m⁻³ was added to the modeled concentrations to ensure consistency with observations.

For the entire one-year period, the correlation coefficient between annual geometric means of modeled and observed concentrations was R = 0.30, indicating moderate reproducibility of temporal variability. In contrast, the mean log(Model/Obs) was −0.035, corresponding to a Model/Obs ratio of 0.92, demonstrating very good agreement in annual mean concentration levels. When the comparison was restricted to release periods, the correlation improved (R = 0.64), while the mean Model/Obs ratio increased to 1.37, suggesting a tendency toward overestimation associated with uncertainties in local release representation and model resolution near the outlet.

These results indicate that, although the model has limitations in reproducing short-term concentration variability, it reliably reproduces annual mean tritium concentrations that are critical for radiological dose assessment. The present validation demonstrates that the ocean dispersion model used in the prior environmental impact assessment has sufficient reliability for evaluating the dispersion behavior of ALPS-treated water, while highlighting the need for further improvements in the treatment of background concentrations and near-field processes.

How to cite: Tsumune, D., Misumi, K., and Tsubono, T.: Reproducibility of ocean dispersion simulations for ALPS-treated water release off Fukushima: comparison with one-year monitoring data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10166, https://doi.org/10.5194/egusphere-egu26-10166, 2026.

The Fukushima Daiichi Nuclear Power Plant (FDNPP) disaster, triggered by the tsunami after the massive earthquake on March 11, 2011, which led to the accumulation of vast quantities of contaminated water used for emergency cooling. Although containment measures were implemented to prevent leakage, the on-site storage facilities approached full capacity. Consequently, Japan announced plans to disposal the Advanced Liquid Processing System (ALPS) treated wastewater, which removes most radionuclides except tritium. TEPCO officially began discharging the treated water on August 24, 2023, diluted with seawater, into the Pacific Coast via a submerged outfall located 1 km offshore at a depth of 13 meters. This decision raised significant concerns among the publics of neighboring countries regarding marine safety. In response, Taiwan established a specialized task force to monitor and to predict the consequences by developing an operational forecast model system to monitor the discharge and provide daily predictions of radioactive dispersion in the Western North Pacific.

The system integrates a three-dimensional hydrodynamic model (CWA-OCM-FH), an extension of the existing operational model CWA-OCM, with a transport model driven by the simulated currents. In order to capture the influence of the Kuroshio Current and the Extension on the transport of tritiated water, the model domain was expanded to 180°E. An unstructured mesh is employed to resolve complex topographic features. The grid resolution varies from approximately 1 km in the coastal zone to less than 20 meters near the discharge outfall, ensuring a representation of spatiotemporal variations in the near-field flow.

To ensure the reliability of the flow fields driving the dispersion, the hydrodynamic model underwent rigorous validation using tide gauge data and ADCP observations. Harmonic analysis on both the observed and simulated data for data for calibration and verification.

Driven by the verified flow fields, a 3D Lagrangian particle tracking model simulates the dispersion pathways of the tritiated water. These computed trajectories provide the essential spatial distribution data required for calculating subsequent concentration. Simulation results indicate that while the primary transport direction follows the Kuroshio Extension and North Pacific Current eastward, mesoscale eddies induce significant cross-stream transport. Therefore, the contaminated particles could potentially influencing waters near Taiwan. 

The model has been verified with observations utilize quantitative metrics such as the Pearson correlation coefficient (R value), coefficient of determination (R²), and Root Mean Square Error (RMSE) over a period exceeding one year. Validation using data from tide gauge stations, ARGO drifter profiles, AVISO satellite altimetry geostrophic currents, and GHRSST sea surface temperature satellite data will be presented and discussed in the paper.

How to cite: Wang, C.-H., Cheng, H.-Y., Yu, J. C. S., Zeng, H.-T., and Teng, J.-H.: An Operational Modeling System Forecasting the Disposal of Fukushima Tritiated Water and Transport: A Lagrangian Particle Tracking System Driven by High-Resolution Hydrodynamics., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14564, https://doi.org/10.5194/egusphere-egu26-14564, 2026.

EGU26-15000 | Posters on site | GI2.5

The Role of Subtropical Mode Water in the Subsurface Transport of Fukushima-derived 137Cs into the South China Sea 

Seung-Tae Lee, Yang-Ki Cho, Kyeong Ok Kim, and Seongbong Seo

The Luzon Strait serves as a critical conduit between the Western North Pacific and the South China Sea (SCS), through which water-mass exchange plays a key role in regulating regional heat budgets and primary productivity. While surface exchange processes have been known well, subsurface intrusion dynamics—particularly those associated with Subtropical Mode Water (STMW)—remain poorly understood. In this study, we investigate the pathways and transport timescales of STMW intrusion through the Luzon Strait by employing radiocesium 137Cs released during the 2011 Fukushima Dai-ichi Nuclear Power Plant (FDNPP) accident as a transient tracer. A three-dimensional Regional Ocean Modeling System (ROMS) was used to simulate the long-term dispersion of 137Cs from the North Pacific into the SCS. The results show that the 137Cs within the STMW layer reached the Luzon Strait approximately seven years after the accident, notably earlier than surface circulation. The net flux of 137Cs into the SCS exhibits seasonal variability, with enhanced inflow during winter, primarily driven by horizontal advection and variations in Kuroshio intrusion behavior. A comparison of different intrusion modes indicates that the leaking path yields a substantially larger net inflow of radiocesium into the SCS than either the looping or leaping paths. Given that the SCS serves as a gateway to downstream marginal seas—including the East China Sea, Yellow Sea, and Japan/East Sea—these findings provide important insights into basin-scale transport processes of Pacific-derived tracers and their potential ecological implications.

How to cite: Lee, S.-T., Cho, Y.-K., Kim, K. O., and Seo, S.: The Role of Subtropical Mode Water in the Subsurface Transport of Fukushima-derived 137Cs into the South China Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15000, https://doi.org/10.5194/egusphere-egu26-15000, 2026.

EGU26-15352 | Orals | GI2.5

Possibility of radionuclide originated from the Fukushima accident as oceanic tracer by fish muscle as bio-indicator 

Yutaka Tateda, Hyoe Takata, Yayoi Inomata, Yasunori Hamajima, and Roman Bezhenar

The Fukushima Dai-ichi Nuclear Power Station (F1NPS) accident released radionuclide was believed to circulate in the North Pacific Ocean and was suggested to arrive at East China Sea ECS (Aoyama et al., 2022). Temporal fraction of 137Cs from F1NPS was estimated to be 0.5 mBq l-1 at ECS in 2023 (Inomata et al., 2023). Appeared 137Cs radioactivity 1.4 mBq l-1 off Okinawa seawater in 2025 seems to suggest still having contribution of 0.6 mBq l-1 as F1NPS originated fraction even after 14 years of the accident, compared to assumed global fallout originated level 0.8 mBql-1 in ECS at 2025 (ENVRDB, 2025). This level was suggested to be caused by recirculation of 137Cs within the north western Pacific waters by Subtropical Mode Water (STMW) and Central Mode Water (CMW)(Kumamoto et al., 2025). Similarly, F1NPS-137Cs may be brought by North Equatorial Current (NEC) within 10-18 years (Chen et al., 2023). However, in contrast, there is other possibility as depuration delay of global fallout-137Cs in surface water by depression of vertical mixing to deeper layer due to high surface water temperature after 2010 as observed global warming. Since F1NPS-orginated 134Cs originated F1NPS almost decayed and being difficult to detect, it is still unknown the precise contribution rate of F1NPS-137Cs compared to global fallout 137Cs fractions. Possible method to derive F1NPS fraction may be using fish muscle which has approximately 50-100 times greater radioactivity in equivalent sample size. Successful detection of F1NPS-originated radio-caesium will is expected not to understand up-to date ocean circulation environment, but also to find the usefulness of bioindicator as oceanic tracer.

How to cite: Tateda, Y., Takata, H., Inomata, Y., Hamajima, Y., and Bezhenar, R.: Possibility of radionuclide originated from the Fukushima accident as oceanic tracer by fish muscle as bio-indicator, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15352, https://doi.org/10.5194/egusphere-egu26-15352, 2026.

EGU26-15358 | ECS | Posters on site | GI2.5

Quantifying groundwater-derived 137Cs fluxes to surrounding coastal waters using radium isotope 

Hiroumi Iino, Daisuke Tsumune, Hiroaki Kato, Nimish Godse, Yuichi Onda, and Shigeyoshi Otosaka

Large amounts of radioactive cesium (134Cs and 137Cs) were released as a result of the Fukushima Daiichi Nuclear Power Plant (F1NPP) accident. Even 15 years after the accident, 137Cs concentrations in the marine environment have not returned to pre-accident levels, indicating that leakage from areas outside of the F1NPP site may still be ongoing.[1] Although 137Cs concentrations in sandy beach groundwater outside the F1NPP site have been reported to be higher than those in seawater, suggesting groundwater as a major leakage pathway, no observational data are available from areas in close proximity to the plant.[2] Based on these considerations, this study aims to estimate discharge flux of 137Cs originating from groundwater in the coastal waters surrounding the F1NPP.

Groundwater-derived 137Cs discharge flux (Bq day-1) was estimated by dividing the inventory (Bq) by the residence time of groundwater (day). Residence times following groundwater discharge to the coastal ocean were estimated using changes in the short-lived radium isotope activity ratios (223Ra/224Ra) between groundwater and seawater. Radium isotopes were selected as groundwater tracers for three reasons: (i) they were scarcely released from the F1NPP, such that the influence of the accident on Ra isotopes can be considered negligible[3]; (ii) radium isotopes (223Ra, 224Ra, 226Ra, and 228Ra) exhibit pronounced concentration differences between groundwater and seawater; and (iii) the wide range of half-lives and multiple isotopes enables their application to the estimation of water residence times as well as to the quantification of nutrient fluxes transported via submarine groundwater discharge.[4] In addition, the spatial area representative of 137Cs leakage for inventory estimation was defined based on the variability of Ra isotopes and 3H. The mean 137Cs concentration within the target domain was determined using seawater sampling data of 137Cs concentrations conducted by Tokyo Electric Power Company Holdings, Inc. (TEPCO HD). The 137Cs inventory (Bq) was then calculated by multiplying the mean 137Cs concentration (Bq m⁻³) by the volume (m³) of the target domain.

The calculated discharge flux is from 2.1×109 to 8.6×109 (Bq day⁻¹). These values are comparable to the flux required to sustain coastal ¹³⁷Cs concentrations (2.0 × 10⁹ Bq day⁻¹)[1], indicating that submarine groundwater discharge may explain why 137Cs concentrations in the vicinity of the FDNPP have not returned to pre-accident levels.

 

[1]Tsumune et al., J Environ Radioact , 2024

[2]Sanial et al., Proc Natl Acad Sci, 2017

[3]Buesselar et al., Ann Rev Mar Sci , 2017

[4]Garcia-Orellana et al., Earth-Science Review, 2021

How to cite: Iino, H., Tsumune, D., Kato, H., Godse, N., Onda, Y., and Otosaka, S.: Quantifying groundwater-derived 137Cs fluxes to surrounding coastal waters using radium isotope, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15358, https://doi.org/10.5194/egusphere-egu26-15358, 2026.

EGU26-15360 | ECS | Posters on site | GI2.5

Radionuclide Dynamics in the Coastal Ocean off the Fukushima Daiichi Nuclear Power Plant Using Radioactivity Ratios. 

Nimish Sudhir Godse, Daisuke Tsumune, Hiroaki Kato, Hiroumi Iino, Yuichi Onda, and Shigeyoshi Otosaka

Fifteen years after the Fukushima Daiichi Nuclear Power Plant (F1NPP) accident, 137Cs and 3H activities in coastal waters near the plant remain elevated compared to surrounding regions, indicating persistent radioactive inputs. While concentrations within the port are highest, recent estimates suggest that the leakage rate outside the port exceeds that inside, implying the presence of an additional or previously unrecognized source outside the F1NPP site. However, the mechanisms governing these releases remain unclear.

The 3H/137Cs activity ratio is a useful tracer for identifying contamination sources, as it remains relatively stable in seawater over short timescales. Since approximately 2016, 137Csconcentrations near the FDNPP have shown little decline, while spatial contrasts in the 3H/137Cs ratio have become more pronounced. Although both radionuclides’ concentrations peak within the port, the ratio is consistently lower there and higher offshore. This suggests the potential existence of sources outside the harbor governing the distribution pattern of the radionuclides.

To investigate these patterns, we applied a color-classified 3H/137Cs ratio analysis and conducted release-rate estimations for the port and adjacent coastal waters. In addition, we collected independent samples of seawater, river water, groundwater, and spring water near the F1NPP. The 3H/137Cs ratios of river water, groundwater, and spring water were used in an end-member mixing analysis to evaluate potential terrestrial and subsurface contributions. Preliminary results indicate that the end members for groundwater and spring water (excluding river water) show trends similar to the 3H/137Csratio in seawater, potentially explaining the observed increase in the ratio offshore.

This integrated analysis improves constraints on radionuclide sources and transport pathways in the F1NPP coastal environment and contributes to a better understanding of long-term radioactive contamination dynamics.

How to cite: Godse, N. S., Tsumune, D., Kato, H., Iino, H., Onda, Y., and Otosaka, S.: Radionuclide Dynamics in the Coastal Ocean off the Fukushima Daiichi Nuclear Power Plant Using Radioactivity Ratios., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15360, https://doi.org/10.5194/egusphere-egu26-15360, 2026.

 The size distribution (SZ) of radioactive aerosols emitted after nuclear accident at nuclear power plants plays a crucial role in assessment of the subsequent atmospheric transport and deposition. However, in reality this distribution in the source is usually unknown. The SZ of particles in the plume also changes with travel time of the plume, because the coarser particles fall out more rapidly than the finer particles. Hence when the measurements of SZ are undertaken at certain distances from the source the SZ could be already altered by plume travel time while it is SZ in the source which is required by atmospheric transport models (ATMs) for simulation of radionuclides atmospheric dispersion and deposition. Also, SZ measurements are usually not available in real time during the accident. More readily available measurements are airborne concentrations. Hence when concentration measurements are available, the SZ parameters of ATMs could be fitted to achieve better agreement between model and measurements.

 In this work, the inverse problem is stated to identify the optimal set of size distribution parameters of the Fukushima source term – activity-averaged mean aerodynamic diameter (d) and geometric standard deviation (σ) which best fit results of FLEXPART ATM to both, local and global measurements datasets. The problem is formulated as multi-objective optimization in which two objective functions. The first objective function J1 corresponds to model deviations from measurements in the territory of Japan, while the second objective function J2 corresponds to model deviations from the global observations of CTBTO measurement stations. The combined cost function J=J1J2 , characterizing model deviation against measurements in both datasets was also considered. In this way, the estimate of the unknown SZ parameters, which fits both local and global concentration observations is to be found. The method of finding Pareto solution of such multi-objective optimization problem was developed and preliminary results of comparisons of the estimated SZ parameters with SZ measurements, performed following Fukushima accident were obtained.

 The solution of the stated problem leads to reasonable results. The simulations with small values of 1≤σ≤2 led to excellent agreement of estimated mean aerodynamic diameter d of emitted particles between 2 and 3 μm with available measurements of SZ. At the same time if large values of σ were allowed the resulting estimated mean aerodynamic diameter could significantly deviate from the observed values. The use of the small values of mean aerodynamic diameter (d <1μm) in turn did not allow for the minimization of the combined cost function J.

How to cite: Jung, K. T., Kim, J.-H., and Kovalets, I.: Inverse estimation of size-distribution parameters of emitted aerosols following the Fukushima accident using FLEXPART simulations and measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15588, https://doi.org/10.5194/egusphere-egu26-15588, 2026.

EGU26-16674 | Posters on site | GI2.5

Deposition of 129I in the forests of Koriyama and 129I/137Cs ratio originated from the Fukushima Daichi Nuclear Power Plant 

Tomoko Ohta, Yasunori Mahara, Hiroyuki Matsuzaki, Hiroshi Hayami, and Daisuke Tsumune

The radionuclides 129I and 137Cs released during the 2011 Fukushima nuclear accident led to contamination of forested environments. The concentrations of these nuclides in precipitation, as well as their subsequent environmental behavior, are critical for assessing internal radiation exposure. In this study, deposition records of atmospheric 129I and 137Cs following the accident were reconstructed using a borehole drilled between 2012 and 2014 at Koriyama, located approximately 60 km from the accident site. After subtraction of contributions from global fallout and nuclear reprocessing facilities, the inventories of 129I and 137Cs in forest soil at Koriyama, integrated to a depth of 50 cm, were estimated to be 4.80 × 105 and 81.7 mBq m−2, respectively. The 129I/137Cs radioactivity ratio derived from Fukushima-derived deposition in litter and soil (0–50-cm depth) was 1.71 × 10−7, which is consistent with the ratio observed in atmospheric aerosols at the time of the accident. The 129I/137Cs radioactivity ratio in the litter layer was marginally lower than that in the underlying topsoil. This difference is attributed to the higher solubility and mobility of 129I relative to 137Cs in litter, resulting in preferential washout from the surface layer. It is therefore inferred that a fraction of 129I originally retained in the litter layer has migrated from the forest surface toward riverine systems.

How to cite: Ohta, T., Mahara, Y., Matsuzaki, H., Hayami, H., and Tsumune, D.: Deposition of 129I in the forests of Koriyama and 129I/137Cs ratio originated from the Fukushima Daichi Nuclear Power Plant, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16674, https://doi.org/10.5194/egusphere-egu26-16674, 2026.

EGU26-17315 | ECS | Orals | GI2.5

Performance Variability of Mid-Infrared Spectroscopy–Based Predictions of Soil Radiocaesium Dynamics across Diverse Soil and Land Use Conditions 

Kazuki Murashima, Jumpei Iwai, Gerd Dercon, Mariana Vezzone, Magdeline Vlasimsky, Franck Albinet, Hayato Maruyama, and Takuro Shinano

Following the Fukushima Daiichi Nuclear Power Plant accident, radioactive substances such as radiocaesium (137Cs) were widely dispersed and contaminated soils, raising concerns about their transfer from soil to crops. 137Cs transfer is primarily regulated by exchangeable potassium (KEx), a chemically analogous element, but its effectiveness varies across environmental conditions such as soil type and land-use. Recent studies suggest that soil exchangeable 137Cs (137CsEx) dynamics and its solid–liquid partitioning play key roles in predicting 137Cs transfer irrespective of regional differences. In contrast, current direct methods for measuring 137Cs are costly and time-consuming, making them unsuitable for rapid risk assessment. As an alternative approach for risk management, mid-infrared spectroscopy (MIRS) may provide a rapid and cost-effective means of estimating soil properties. Recently, models for predicting soil KEx concentrations from spectral data have been reported. However, their applicability to 137Cs transfer remains unclear. In this study, we aimed to construct prediction models for the ratio of soil 137CsEx to soil total 137Cs (137CsTotal) using MIRS spectra and to evaluate the variability of model performance among soil or land-use categories.

1249 soil samples collected in Fukushima Prefecture, Japan, from 2015 to 2020, were analyzed for soil properties, including soil total C, 137CsEx, and 137CsTotal, through MAFF and NARO in Japan. Each soil sample was analysed after drying at 37°C for at least 12 hours and being sieved to less than 0.2 mm before measurement. Mid-infrared spectra for these samples were obtained at the FAO/IAEA Soil and Water Management and Crop Nutrition Laboratory over the wavenumber range of 650–4000 cm–1 using four replicate measurements per sample. Using noise-removed spectral data, partial least squares regression models were developed to predict the ratio of soil 137CsEx to 137CsTotal. In addition, prediction models were constructed for different soil types (andosol, brown forest soil, lowland soil, and peat soil) and land-use categories (upland fields and paddy fields), and their differences in model performance were evaluated.

Prediction models were constructed and achieved moderate predictive performance (R² around 0.6). In contrast, by stratifying prediction models by soil type, prediction accuracy improved for all soil types except for peat soil relative to the non-stratified model. In particular, andosol showed the highest prediction accuracy. Comparison of variable importance in projection (VIP) scores among these models showed that the contributions of specific wavenumber ranges to model performance differed among soil types. In andosols, VIP scores were higher in wavenumber ranges associated with carbohydrates, quartz, and clay minerals compared with the model constructed using all data. These results suggest that soil type specific mineralogical composition and carbon content may play roles in improving prediction performance. Furthermore, predictions stratified by land-use showed higher accuracy in upland fields than in paddy fields. Differences of VIP scores between them were also observed in wavenumber ranges associated with carbohydrates and clay minerals. These results suggest that environmental conditions, such as soil redox status, may influence prediction accuracy through their effects on soil minerals and carbon.

How to cite: Murashima, K., Iwai, J., Dercon, G., Vezzone, M., Vlasimsky, M., Albinet, F., Maruyama, H., and Shinano, T.: Performance Variability of Mid-Infrared Spectroscopy–Based Predictions of Soil Radiocaesium Dynamics across Diverse Soil and Land Use Conditions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17315, https://doi.org/10.5194/egusphere-egu26-17315, 2026.

EGU26-18568 | Orals | GI2.5

Why Are Dissolved ¹³⁷Cs Concentrations Lower in Fukushima Rivers? A Comparative Study with European Catchments 

Yuichi Onda, Yasunori Igarashi, Jim Smith, Aya Sakaguchi, Shaoyan Fan, and Junko Takahashi

Nuclear accidents contaminate large terrestrial areas with long-lived radionuclides, and river systems play a key role in their redistribution. The concentration of dissolved radiocaesium (¹³⁷Cs) in river water is influenced by catchment-scale physical and geochemical characteristics. After the Chernobyl accident, environmental radionuclide concentrations generally declined over time; however, systematic inter-river comparisons remain limited, and the key factors controlling long-term differences in dissolved ¹³⁷Cs concentrations are still poorly understood.

In this study, we investigated the environmental behavior of dissolved ¹³⁷Cs in river systems affected by the Fukushima Daiichi Nuclear Power Plant accident and compared it with long-term observations from major European rivers impacted by the Chernobyl accident. In Fukushima, river water samples were seasonally collected between 2021 and 2024 from headwater catchments in the Yamakiya and Kuchibuto River basins. Samples were filtered through 0.22 µm membranes, and dissolved ¹³⁷Cs was measured using high-purity germanium detectors. Major ions (K⁺, NH₄⁺), stable ¹³³Cs, and dissolved organic carbon (DOC) were also analyzed. Univariate and multivariate regression analyses were applied to identify dominant release mechanisms. Catchment land cover, topographic gradients, and precipitation were analyzed using GIS, and groundwater residence times were estimated. These results were compared with long-term monitoring data and additional field measurements from nine European river catchments in Ukraine, Finland, Austria, and Italy, incorporating climatic, vegetation, and anthropogenic factors into an international comparison framework.

In Fukushima headwater catchments, dissolved ¹³⁷Cs concentrations increased from summer to autumn, coinciding with rising temperatures, enhanced organic matter decomposition, and increased K⁺ availability. Multiple regression analysis identified ¹³³Cs and K⁺ as significant explanatory variables, indicating that ion exchange plays a key role in ¹³⁷Cs mobilization. In contrast, DOC showed only a weak relationship with ¹³⁷Cs in Fukushima rivers. Comparative analysis of dissolved ¹³⁷Cs trends since 1986 revealed that European rivers have maintained higher concentrations over longer periods. Correlation analysis demonstrated that DOC and ¹³³Cs were significant scaling factors controlling dissolved ¹³⁷Cs concentrations across European river systems, whereas K⁺ and NH₄⁺ contributed little to concentration variability.

These results indicate that differences in the long-term behavior of dissolved ¹³⁷Cs between Fukushima and European rivers are associated with contrasting DOC- and ¹³³Cs-related controls at the catchment scale. This study suggests that accounting for regional variability in biogeochemical controls should be useful for long-term river environment and also can inform environmental modeling of radionuclide transport under nuclear emergency conditions, contributing to improved preparedness and long-term risk assessment.

How to cite: Onda, Y., Igarashi, Y., Smith, J., Sakaguchi, A., Fan, S., and Takahashi, J.: Why Are Dissolved ¹³⁷Cs Concentrations Lower in Fukushima Rivers? A Comparative Study with European Catchments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18568, https://doi.org/10.5194/egusphere-egu26-18568, 2026.

EGU26-22532 | Posters on site | GI2.5

Developing Ontology-Based Nuclear Accident Knowledge Base 

Misa Yasumiishi and Thoma Bittner

The society acquired vast amounts of data from past major nuclear accidents, then learned the causes of those accidents, the methods to mitigate their adverse effects, and accident-prevention measures. However, it is challenging to store and organize highly technical knowledge related to nuclear accidents and share it in ways that meet our purposes. That is one reason we still do not have a centralized public database of nuclear incidents, despite efforts by international organizations such as the IAEA and academic institutions. Internet searches and AI queries return answers based on publicly available data sources without curation, thereby posing a risk of biased knowledge representation.

We aim to develop a prototype nuclear accident knowledge base using an ontology-based approach to establish the structured management system of nuclear accident-related knowledge. The top-level classes of the Basic Formal Ontology (BFO) are reviewed and utilized to design the base ontology hierarchy of the entities involved in nuclear accidents. The past ontology work in the nuclear and non-nuclear industries is reviewed, and some of their proposed classes and relationships were imported into the nuclear accident knowledge base structure. The classes, entities, and relations among those entities, and data properties relevant to the knowledge base are defined and are entered in protégé ontology editing software, whose ontology design can be shared digitally with interested parties.

During the development of the ontology structure, five knowledge-ambiguity factors were identified as potential focal points for developing the nuclear accident knowledge base. The ambiguity factors include: 1) terminology definition, 2) location definition, 3) temporal change in knowledge needs, 4) contamination definition, and 5) accident cause definition. When sharing nuclear accident knowledge, these factors must be considered to minimize confusion during the user’s knowledge-finding endeavour. By dissecting those ambiguity factors and providing a logical structure for nuclear accident-related data, this prototype knowledge base will assist in developing a public centralized nuclear accident knowledge base that can serve as a trustworthy data depository for preventing future accidents as well as enabling prompt recovery from the adverse effects of those accidents.

 

References.

Arp, R., Smith, B., Spear, A.D., 2015. Building ontologies with basic formal ontology. Mit Press. https://doi.org/10.7551/mitpress/8743.003.0011

Booshehri, M., Emele, L., Flügel, S., Förster, H., Frey, J., Frey, U., 2021. Introducing the open energy ontology: Enhancing data interpretation and interfacing in energy systems analysis. Energy and AI 2021; 5: 100074. https://doi.org/10.1016/j.egyai.2021.100074

Rashdan, A., Browning, J., Ritter, C., 2019. Data Integration Aggregated Model and Ontology for Nuclear Deployment (DIAMOND): Preliminary Model and Ontology. Idaho National Laboratory. https://doi.org/10.2172/2439922

Sorokine, A., Schlicher, B.G., Ward, R.C., Wright, M.C., Kruse, K.L., Bhaduri, B., Slepoy, A., 2015. An interactive ontology-driven information system for simulating background radiation and generating scenarios for testing special nuclear materials detection algorithms. Engineering Applications of Artificial Intelligence 43. 157-165. https://doi.org/10.1016/j.engappai.2015.04.010

U.S. Department of Energy, 2022. Environmental Radiological Effluent Monitoring and Environmental Surveillance.

How to cite: Yasumiishi, M. and Bittner, T.: Developing Ontology-Based Nuclear Accident Knowledge Base, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22532, https://doi.org/10.5194/egusphere-egu26-22532, 2026.

EGU26-2950 | ECS | PICO | ESSI1.7

Predicting Cumulative Land Subsidence and Its Spatiotemporal Relationship Using Machine Learning 

Yu-Yun Hsu, WeiCheng Lo, Jhe-Wei Lee, and Chih-Tsung Huang

Land subsidence has long been a critical environmental hazard along the southwestern coast of Taiwan, with Yunlin County being one of the most severely affected areas. In this study, Long Short-Term Memory (LSTM) neural networks are employed to develop predictive models for land subsidence. Cumulative land subsidence, groundwater-level variations, and lithological layering are considered as input features to investigate the predictive performance of the models from both temporal and spatial perspectives.

As long-term groundwater monitoring data often suffer from missing values, this study further introduces a Cue Wasserstein GAN with Gradient Penalty (CWGAIN-GP) to impute missing groundwater-level data, thereby improving the stability and completeness of subsequent prediction models. Artificial masking experiments, including continuous missing periods ranging from one month to one year and random removal of 10%–50% of the data. The results show that the average Nash–Sutcliffe efficiency (NSE) achieved by the imputation model reaches 0.897.

For temporal prediction, the land subsidence model is trained using different training lengths (one year and seven years) and variable combinations to forecast cumulative land subsidence over the following one to two years. The most recent six months of observations are used as input to predict the monthly land subsidence increment. The results indicate that longer training periods and more comprehensive input variables lead to improved model performance. The coefficient of determination (R²) for the first prediction year reaches 0.945, while for the second year—under conditions of three consecutive months of missing data—the R² remains as high as 0.923.

For spatial prediction, a multi-station training and single-station validation strategy is adopted. When predicting a target station, the three nearest neighboring stations are selected, and their observations from the most recent three months are used as inputs to predict the monthly land subsidence increment at the target station. This increment is then combined with the known cumulative subsidence from the previous month to estimate the current cumulative subsidence. The results show that the average R² for single-month predictions reaches 0.966. Even when cumulative subsidence is estimated iteratively by adding predicted monthly increments over six consecutive months, the average R² remains around 0.90, demonstrating strong spatial generalization capability of the proposed model.

Fig.1 Monthly vertical profiles of cumulative land subsidence at different depths for the Huwei (MW_HWES) station in 2021.

Overall, this study demonstrates that cumulative land subsidence can be effectively predicted by integrating temporally and spatially informed LSTM models with vertically stratified hydrogeological information. Although cumulative subsidence is used as the primary prediction target, the inclusion of groundwater-level variations and lithological layering enables the model to capture the vertical characteristics of aquifer systems and their influence on subsidence processes. The results highlight the importance of incorporating stratified subsurface information when modeling land subsidence and provide a robust framework for spatiotemporal subsidence prediction under realistic data availability constraints.

How to cite: Hsu, Y.-Y., Lo, W., Lee, J.-W., and Huang, C.-T.: Predicting Cumulative Land Subsidence and Its Spatiotemporal Relationship Using Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2950, https://doi.org/10.5194/egusphere-egu26-2950, 2026.

Soil moisture downscaling is a challenging geospatial regression task that requires accurately capturing complex spatiotemporal relationships across scales. In this study, we conduct a preliminary applicability assessment of denoising diffusion probabilistic models (DDPMs) for continuous-value geospatial regression, exploring the potential of generative modeling frameworks for soil moisture downscaling. The model learns the relationships between coarse-resolution soil moisture observations and multi-source auxiliary features, enabling the generation of high-resolution soil moisture estimates.

During training, the model uses 36 km resolution satellite soil moisture data and conditions on auxiliary variables, including normalized difference vegetation index (NDVI), land surface temperature, surface albedo, precipitation, and digital elevation model (DEM). A conditional embedding strategy is introduced to incorporate temporal information, spatial location information, and in-situ statistics into the diffusion network via feature-wise linear modulation (FiLM), enhancing the model’s ability to capture complex spatiotemporal structures while maintaining stability. During inference, a two-stage “generation–correction” pipeline is employed: high-resolution (1 km) auxiliary features are first used to generate initial predictions through the diffusion model, which are subsequently bias-corrected using in-situ station data.

The applicability assessment combines quantitative and qualitative evaluation. Quantitative metrics include unbiased mean squared error (UMSE), root mean square error (RMSE), mean absolute error (MAE), and R², while qualitative evaluation focuses on spatial pattern consistency and temporal trend representation. Experimental results indicate that the diffusion-based generative model produces reasonable, spatially coherent, high-resolution soil moisture results and successfully captures major temporal variations. These findings demonstrate the applicability of generative frameworks for geospatial regression and their potential as a geospatial regression modeling paradigm, providing a foundation for further refinement and evaluation.

How to cite: Yu, X., Hu, L., Su, C., Yan, Y., Wu, S., and Du, Z.: Long-term Soil Moisture Downscaling Based on Diffusion Models: Applicability Assessment of Generative Models for Geospatial Regression Tasks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5255, https://doi.org/10.5194/egusphere-egu26-5255, 2026.

EGU26-8056 | ECS | PICO | ESSI1.7

Global Sensitivity Analysis of Spatial Interpolation for Sparse, Clustered, and Censored Data: A Case Study of Groundwater Sulfate in the Paris Basin 

Corinna Perchtold, Jeremy Rohmer, Augustin Thomas, Julie Lions, and Martin Wieskotten

This study presents a comprehensive sensitivity analysis framework to disentangle the drivers of predictive uncertainty in spatial interpolation and how they ultimately affect spatial predictions. Developed within a Global Sensitivity Analysis context, the proposed approach is model-independent and generic, allowing for broad application across diverse spatial interpolation workflows.

The framework is demonstrated using groundwater Sulfate concentration in the Paris Basin, a dataset characterised by sparse and highly clustered sampling across six distinct aquifers according to the French "BD LISA" hydrogeological system (https://bdlisa.eaufrance.fr/). We represent the underlying spatial process as a  Gaussian Random Field, leveraging Integrated Nested Laplace Approximations for computationally efficient Bayesian inference. This allows for a  probabilistic treatment of uncertainty even within complex spatial structures.

We systematically evaluate the impact of several key uncertainty factors related to both data and model configuration: (1) the number of monitoring stations and their spatial distribution; (2) the selection of the environmental covariates  and the functional form of their effects (linear vs. non-linear); (3) the treatment of censored data (values below detection limits); and (4) structural assumptions regarding the spatial covariance function, specifically the estimation of variogram hyperparameters such as range, sill, and nugget effects and their prior specification. By propagating these uncertainty sources through our framework, we derive domain-wide aggregated sensitivity measures. These metrics quantify how specific data topologies—including sampling density, clustering effects, and censoring rates—govern the stability and accuracy of the resulting spatial interpolations.

Finally, the results facilitate an in-depth discussion on the limitations of purely probabilistic methods in data-poor scenarios. We provide an outlook on the potential of extra-probabilistic approaches, such as imprecise or interval-based kriging, to more robustly address the wide range of epistemic uncertainties inherent in environmental monitoring.

We acknowledge financial support of the French National Research Agency within the HOUSES project (grant N°ANR-22-CE56-0006).

How to cite: Perchtold, C., Rohmer, J., Thomas, A., Lions, J., and Wieskotten, M.: Global Sensitivity Analysis of Spatial Interpolation for Sparse, Clustered, and Censored Data: A Case Study of Groundwater Sulfate in the Paris Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8056, https://doi.org/10.5194/egusphere-egu26-8056, 2026.

Predicting building attributes—such as functional classification, socioeconomic status, and energy efficiency—is a fundamental task in urban science. The current paradigm involves leveraging domain knowledge to extract attribute-specific morphological or topological features for supervised modeling. However, this heavy reliance on manual feature engineering often leads to task-specific models where features must be redefined for each attribute. Consequently, the field lacks a unified, generalizable framework capable of multi-attribute building prediction.

Inspired by recent advances in Regression Language Models (RLMs), which cast continuous prediction as a text-to-text task, we propose Buildings as Text (BaT). BaT serializes structured building representations (e.g., GeoJSON) into raw text and enables end-to-end text-to-text regression. To mitigate the spatial sensitivity of building data, we introduce a Topology-Preserved Coordinate (TPC) strategy that removes each building text’s absolute positional information. Specifically, TPC applies a global coordinate shift to the serialized geometry, suppressing absolute-location bias while preserving local shape and topology. By operating directly on raw text, BaT eliminates manual feature engineering and allows the model to learn a “spatial syntax” from the underlying geometric descriptions.

We validated the BaT framework through a case study on informal settlement (slum) classification. The results demonstrate that our model achieves superior performance and higher adaptability compared to traditional morphology-based methods. While validated on slum detection, this research offers a universal and scalable paradigm for urban building analysis, suggesting that Large Language Models can effectively "read" urban forms for diverse prediction tasks beyond specific domains.

How to cite: Wang, C.-C. and Luo, P.: Buildings as Text: A Universal Regression Paradigm for Building Attribute Prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8402, https://doi.org/10.5194/egusphere-egu26-8402, 2026.

EGU26-11193 | ECS | PICO | ESSI1.7

A preliminary study of the morphology and spatial distribution of funerary elements in Oman 

Ana Sofia Meneses Pineda, Marco Solinas, Marco Ramazzotti, Massimo Musacchio, and Maria Fabrizia Buongiorno

The archaeological landscapes of northern Oman host thousands of funerary monuments of different periods and morphologies, forming one of the densest and least explored burial regions of the Arabian Peninsula. Within the framework of LAA&AAS (Laboratorio di Archeologia Analitica e Sistemi Artificiali Adattivi) and MASPAG (Missione Archeologica della Sapienza nella Penisola Arabica e nel Golfo), a multidisciplinary project supported by Sapienza University of Rome and the Italian Ministry of Foreign Affairs, we developed a reproducible geo-AI workflow to classify and analyse funerary structures based on remote-sensing and spatial-context information.

The first dataset, encompassing 185 tombs mapped in the Southwestern Cemetery near the village of Muslimat, in the region of Wadi al-Maʿawil (ca. 70 Km southwest of Muscat) was used to test a machine-learning pipeline designed to discriminate between morphological classes (“tombs” vs “non-tombs”, and within-type subclasses) from high-resolution satellite imagery and derived spatial metrics. Two Random Forest models were compared: a geometry-only baseline using shape descriptors (area, compactness, circularity, elongation), and an extended model incorporating spatial-context features such as kernel density, nearest-neighbour distances, Moran’s I local autocorrelation and cluster membership. The integration of these contextual descriptors increased overall accuracy from 59 % to 76 %, improving model reliability and reducing false positives in morphologically ambiguous contexts. The workflow includes systematic feature importance analysis and confusion-matrix evaluation to assess interpretability and class-imbalance effects.

Beyond the single-site test case, this approach aims to address a broader spatiotemporal challenge: learning and transferring morphological–contextual patterns across different archaeological regions. During 2025 field campaign (20 October – 20 December 2025), more than 500 new tombs were surveyed and georeferenced in the area of the Western Cemetery, expanding the available dataset and enabling large-scale testing of model scalability and transferability. This new phase will assess whether models trained in Wadi al-Maʿawil can generalize to nearby valleys with comparable geomorphological and cultural settings, supporting semi-automated mapping and predictive modelling of funerary features.

The presented pipeline, implemented in an open-source environment (Python, QGIS, and scikit-learn), is designed for reproducibility and transparent parameter tracking. All processing steps—from data preparation and feature extraction to model training and evaluation—are logged and versioned, facilitating cross-project reuse. The workflow thus bridges archaeological and geospatial domains, demonstrating how spatially aware machine learning can improve the detection, classification, and interpretation of complex cultural landscapes.

This contribution highlights the potential of AI and ML in managing spatiotemporal archaeological data and in advancing reproducible analytical frameworks. The methodological approach developed for the Omani funerary landscapes can be generalized to other MASPAG regions, supporting comparative analysis of desert landscapes and long-term dynamics of human–environment interaction across the Arabian Peninsula.

How to cite: Meneses Pineda, A. S., Solinas, M., Ramazzotti, M., Musacchio, M., and Buongiorno, M. F.: A preliminary study of the morphology and spatial distribution of funerary elements in Oman, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11193, https://doi.org/10.5194/egusphere-egu26-11193, 2026.

EGU26-11342 | PICO | ESSI1.7

Using Moran's I for assessing residual spatial autocorrelation in machine learning models  

Jakub Nowosad, Hanna Meyer, and Jonas Schmidinger

Understanding the spatial dependence of residuals is important for interpreting and diagnosing spatial machine learning models. Spatial autocorrelation in the residuals suggests that the model has not fully captured the data's spatial structure. This may imply that the model is missing crucial spatial context or interactions, and that, in effect, it is spatially biased, leading to underestimation in some areas and overestimation in others.

Moran's I is a commonly used statistic for the diagnosis of spatial autocorrelation in spatial predictions, providing a single-value quantitative measure with a straightforward interpretation. This measure quantifies the degree of spatial autocorrelation, indicating whether similar values are clustered together or dispersed across space. The information provided by Moran's I has been used in various ways in studies applying machine learning: to evaluate model performance, interpret results, understand model limitations, and compare different modeling approaches.

Unlike standard model performance metrics, such as R2 or RMSE, Moran's I depends not only on the values of residuals but also on the spatial contextespecially the study area's extent, the sampling strategy used, and the specification of spatial weights. However, there is a lack of a comprehensive understanding of how these factors influence the results of Moran's I calculation in the context of spatial machine learning, and of how to best use this measure for model evaluation and comparison.

Using simulated data with controlled spatial properties, we investigated how testing set size, sampling strategy, and the specification of spatial weights influence Moran's I computed on model residuals. Our results show that Moran's I, calculated based on k-nearest neighbors approach,  primarily reflects the spatial structure of values in the testing set rather than the residual autocorrelation across the full prediction domain, often underestimating fine-scale spatial patterns. These findings have various implications: weight-matrix definitions must be clearly reported, calculations on sparsely distributed or clustered samples should be avoided, Moran's I is generally not directly comparable across studies due to differences in spatial extents and sampling, and its values are inherently scale-dependent.

With this contribution, we aim to present the behavior of Moran's I calculated from residuals of spatial machine learning models under different conditions, outline best practices for selecting and reporting spatial weights, and discuss how to interpret Moran’s I. 

 

 

How to cite: Nowosad, J., Meyer, H., and Schmidinger, J.: Using Moran's I for assessing residual spatial autocorrelation in machine learning models , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11342, https://doi.org/10.5194/egusphere-egu26-11342, 2026.

EGU26-12275 | ECS | PICO | ESSI1.7

Area of Applicability for Deep Learning: Exploring Latent Space Geometry of Earth Observation Models 

Darius A. Görgen, Simon Heilig, Lara Meyn-Grünhagen, Asja Fischer, Johannes Lederer, and Hanna Meyer

Machine learning methods are used ubiquitously within the Earth Sciences to model spatio-temporal phenomena. These methods scale very well to big data sets and are used to model complex non-linear relationships between the predictor and outcome variables. Yet, most methods might silently fail when used in extrapolation scenarios, e.g. when combinations of predictor variables are encountered that have not been seen during training. This might be the case when the model is applied to new geographic areas that differ from the areas the model was trained on. For traditional machine learning models, estimating the area of applicability based on distances in the predictor space has been proposed. New inputs with distances above a certain threshold are rejected from prediction since our confidence in the model's output is low and we do not expect the estimated performance to hold.

Inspired by the success of deep architectures in the field of computer vision, the use of deep neural networks has been steadily increasing, especially in Earth Observation. Translating the concept of the area of applicability to deep architectures, however, remains a open research challenge. For the safe deployment of such models in the real world it is required to flag inputs for which we expect the model to extrapolate and is thus operating outside the estimated performance measure.

In this work, we are extending the concept of the area of applicability to deep neural network architectures. As an application rooted in current practices for Earth Observation, we use networks trained end-to-end for scene classification. We use these models as feature extractors to obtain representations of input samples in embedding space. We derive the area of applicability of the model within this space based on distances between training and calibration samples. For this purpose, we test different distance measures (euclidean, mahalanobis), leveraging the concept of KNN-distances, which also takes local point densities into account and test whether principal components of the embeddings improve the delineation of the area of applicability.

Our results highlight practical relevant trade-offs between different distance metrics operating in high-dimensional embedding spaces to derive the area of applicability for deep neural networks. The methodology presented can serve as a baseline to ensure the reliability of deployed models in safety critical applications.

How to cite: Görgen, D. A., Heilig, S., Meyn-Grünhagen, L., Fischer, A., Lederer, J., and Meyer, H.: Area of Applicability for Deep Learning: Exploring Latent Space Geometry of Earth Observation Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12275, https://doi.org/10.5194/egusphere-egu26-12275, 2026.

Near-real-time forest monitoring is a critical component for managing climate risk and resource conservation in the Brazilian Legal Amazon (ALB). The DETER program, managed by the National Institute for Space Research (INPE), has played a pivotal role for over two decades by producing warnings of deforestation and forest degradation to support environmental enforcement by agencies such as IBAMA. However, the effectiveness of these warnings is highly dependent on temporal efficiency — the speed at which a disturbance is detected and published after the activity begins.

Recent objective evaluations of DETER’s performance regarding selective logging — a major driver of forest degradation — revealed a significant median delay of approximately 312 days between the start of logging activities and the corresponding warning publication during 2022-2023. This temporal gap highlights the challenge of applying traditional monitoring to complex spatiotemporal datasets, where factors like cloud cover and sensor resolution can hinder early detection.

To address these challenges, this research proposes a novel approach within the framework of AI and Machine Learning in Spatiotemporal Contexts. We leverage Foundation Models and Deep Learning architectures designed to process the complex temporal dynamics of tropical forests using Harmonized Landsat-Sentinel (HLS) time series. A key contribution of using foundation models in this pipeline is their ability to learn robust representations from large-scale data, significantly reducing the requirement for vast volumes of manually annotated samples — a known bottleneck for AI-based remote sensing monitoring systems. By applying these models to HLS data, we aim to improve spatiotemporal predictions and the reliability of the modeling pipeline, facilitating the production of more agile and efficient early warnings.

This work contributes to the development of the next generation of forest monitoring systems, focusing on interpretability and transferability across the Amazonian landscape. By reducing the detection lag of selective logging, this approach seeks to enhance technological sovereignty in environmental monitoring and provide more effective decision-making support for forest preservation.

How to cite: Taquary, E. and Aragão, L.: Enhancing Near-Real-Time Forest Monitoring: Foundation Models and Harmonized Landsat-Sentinel (HLS) Time Series for Selective Logging Detection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16001, https://doi.org/10.5194/egusphere-egu26-16001, 2026.

EGU26-19025 | ECS | PICO | ESSI1.7

A framework for assessing the quality of spatial data applied in supervised image classification of deprived urban areas 

Florencio Campomanes V, Monika Kuffer, Alfred Stein, Anne M. Dijkstra, Lorraine Trento Oliveira, and Mariana Belgiu

The integration of Earth Observation (EO) data with machine learning (ML) has transformed the mapping of Deprived Urban Areas (DUA). Despite these technical advances, persistent disconnect remains between research outputs and their operational uptake by local stakeholders. In parallel, advances in ML and deep learning (DL), together with new satellite missions have improved the extraction of building footprints and urban morphology. Nevertheless, DUA mapping studies, which largely depend on these physical indicators, often prioritize benchmark performance over the robustness, transparency, or usability required in real-world decision-making contexts. One of the main reasons for this gap is spatial data quality (SDQ), which fundamentally limits model performance and generalization. When data quality is poor, due to inaccuracies, incompleteness, or inadequate provenance, models become unreliable, regardless of architectural complexity. Furthermore, many studies rely on validation strategies that ignore spatial autocorrelation, thereby yielding overoptimistic accuracy estimates that mask poor generalization to new local contexts.

To address these challenges, this paper argues for a shift toward a systematic assessment of spatial data quality. We first conduct a scoping review of 50 state-of-the-art DUA mapping studies published between 2017 and 2025. Our analysis reveals a high dependence on very-high-resolution imagery (72%), a widespread lack of publicly accessible data and code (92%), and a critical deficiency in operationalizing semantic definitions of DUAs with 90% of studies failing to provide mapping rules (for visual interpretation) or ground rules (for in-situ collection). Most studies also fail to assess user needs (90%) or do not consider the ethical implications of using DUA data (88%), which is highly sensitive due to risks such as forced evictions. Building on these findings and established international standards from ISO and the OGC, we propose a comprehensive Spatial Data Quality (SDQ) framework tailored to transparently document supervised image classification in DUA mapping. This framework integrates established practices such as adherence to the Findable, Accessible, Interoperable, Reusable (FAIR) principles and assessment of acquisition, measurement and spatial-temporal quality with novel dimensions addressing semantic consistency, sampling representativeness, human factors in annotation, learning shortcut risk, user needs validity, ethical considerations, and transparent reporting of the dataset’s potential failure modes or uncertainties. By operationalizing SDQ as a living, extensible framework, this work aims to better align advances in ML and DL with sustained societal impact, ensuring that DUA mapping products, or any relevant application domain, are fit for use by local communities and decision-makers.

How to cite: Campomanes V, F., Kuffer, M., Stein, A., Dijkstra, A. M., Trento Oliveira, L., and Belgiu, M.: A framework for assessing the quality of spatial data applied in supervised image classification of deprived urban areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19025, https://doi.org/10.5194/egusphere-egu26-19025, 2026.

EGU26-19057 | ECS | PICO | ESSI1.7

Satellite imagery for greenhouse mapping in Morocco using U-net model 

Said El hachemy, Chaima Aglagal, Hamza Ait-Ichou, Ilham Elhaid, Jawad Zlaiga, Mohammed Hssaisoune, Lhoussaine Bouchaou, and Salwa Belaqziz

Greenhouse agriculture has become a crucial element of agricultural practices in Morocco, yet its spatial and temporal evolution remain insufficiently quantified. This study aims to map greenhouse structures at the Souss-Massa region scale in order to assess the progress of covered agriculture and examine its relationship with socio-economic development in Morocco. Using hand-annotated greenhouse data from the Chtouka region as ground truth, we develop a deep learning–based detection framework relying exclusively on open-source tools. Multispectral Sentinel-2 satellite imagery at 10 m spatial resolution is used as input to a U-Net convolutional neural network, which is trained, validated, and tested for greenhouse segmentation. The proposed model achieves an overall accuracy of up to 94%, demonstrating strong generalization capability. The resulting plug-and-play methodology enables scalable, cost-effective, and open-source greenhouse mapping, and provides valuable insights into the dynamics of covered agriculture and its role in Morocco’s agricultural and socio-economic development.

How to cite: El hachemy, S., Aglagal, C., Ait-Ichou, H., Elhaid, I., Zlaiga, J., Hssaisoune, M., Bouchaou, L., and Belaqziz, S.: Satellite imagery for greenhouse mapping in Morocco using U-net model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19057, https://doi.org/10.5194/egusphere-egu26-19057, 2026.

EGU26-19452 | ECS | PICO | ESSI1.7

Improving Dengue Forecasting with Spatiotemporal Data Augmentation and Machine Learning 

Negar Siabi, Rackhun Son, Maik Thomas, Christopher Irrgang, and Jan Saynisch Wagner

Accurate forecasting of vector-borne diseases such as dengue is often challenged by limited and noisy spatiotemporal data. This study evaluates the effectiveness of data augmentation techniques in enhancing the robustness and predictive accuracy of machine learning models. We assess multiple augmentation strategies applied to weekly dengue case data across countries in South and Central America (2014–2022). Results show that augmentation substantially improves short-term forecasting performance, particularly in regions with sparse or irregular observations, yielding higher R² values and lower relative errors compared to non-augmented baselines. These findings demonstrate that well‑designed augmentation can mitigate data scarcity and strengthen the generalization of graph‑based deep learning frameworks for epidemiological forecasting. Overall, the study highlights augmentation as a practical and scalable approach for improving spatiotemporal ML applications in disease surveillance.

How to cite: Siabi, N., Son, R., Thomas, M., Irrgang, C., and Saynisch Wagner, J.: Improving Dengue Forecasting with Spatiotemporal Data Augmentation and Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19452, https://doi.org/10.5194/egusphere-egu26-19452, 2026.

EGU26-19669 | ECS | PICO | ESSI1.7

A Two‑Stream Spatiotemporal Architecture with Foundation‑Model Features Applied to Crop Classification 

João Gabriel Vinholi, Rim Sleimi, Florian Werner, and Albert Abelló

At continental scale, crop classification needs models that capture phenology through temporal analysis without degrading field boundaries. We introduce a decoupled architecture that uses static foundation‑model features across multi‑sensor time series and fuses them with high‑resolution spatial features. The temporal stream ingests paired multispectral and SAR sequences plus a static DEM and metadata, extracts foundation model token features per timestep, and compresses them with a Perceiver‑style bottleneck that cross attends from a fixed latent bank to the full foundation model token volume. Such heavy compression collapses sequence length by orders of magnitude, which makes longer temporal windows and larger batches ingestible on consumer‑grade GPU memory constraints while preserving the temporal signatures needed to separate crops with similar single‑date appearance.
The spatial stream stays purely static --- it selects a single high‑quality multispectral reference frame and passes it through a high‑resolution backbone to retain fine geometry and crisp boundaries. The two streams are joined in a query‑based decoder, where dynamic queries generated from the compressed temporal latents attend to multi‑scale spatial features, aligning phenological signatures with precise field edges. This fusion mechanism prevents coarse temporal features from blurring geometry and makes delineation robust to shifts in timing or crop management practice. In fact, temporal queries encode crop‑specific growth signatures, while the spatial stream supplies the pixel‑level evidence for boundary localization, whereas the decoder enforces instance‑aware segmentation through iterative cross‑attention and masked refinement.
We evaluate on EuroCrops crop‑class labels, achieving a Micro Recall of 84.1% and a Segmentation Quality of 84.2%. Transferability is tested with a spatial holdout protocol using geographically disjoint train/test regions, reliability is summarized by aggregate metrics on these strict splits, and uncertainty is communicated through per‑class performance variability and label‑noise sensitivity analyses that bound achievable scores.

How to cite: Vinholi, J. G., Sleimi, R., Werner, F., and Abelló, A.: A Two‑Stream Spatiotemporal Architecture with Foundation‑Model Features Applied to Crop Classification, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19669, https://doi.org/10.5194/egusphere-egu26-19669, 2026.

EGU26-20221 | ECS | PICO | ESSI1.7

Using Large Language Models to Enhance Spatial Data Discovery in Spatial Data Infrastructures 

James Okemwa Ondieki, Matthes Rieke, and Simon Jirka

Spatial Data Infrastructures (SDIs) contain a lot of spatial data from various organizations and data producers. Metadata is intended to enable the discovery of the data, yet finding the relevant data can be challenging. The challenges include rigid keyword-search, complex search interfaces in geoportals, map-based search that require some geographic knowledge, and language differences between user queries and the metadata.

The development of Large Language Models (LLMs) offers new opportunities to improve spatial data discovery. LLMs demonstrate strong language understanding and generation capabilities and have been used in information retrieval tasks. They can overcome semantic differences and language barriers between user queries and the needed information. However, their internal knowledge is limited and they are prone to hallucinations. Unless the datasets in SDIs, or the web pages describing them are indexed by search engines, LLMs with internet search tools cannot find them. 

Retrieval-Augmented Generation (RAG) offers a solution for the knowledge limitations, by connecting an LLM with an external and up-to-date knowledge base. However, RAG mainly works in the textual domain and excels at retrieving external information that is semantically relevant to a user query. Queries for geographic data have a spatial aspect yet the spatial reasoning capabilities of LLMs are limited. For a query like “forest data for Vienna”, RAG can identify the relevant forest data from a pool of metadata, regardless of the language or words used to describe the data. However, identifying datasets that meet the spatial intent is a problem. DCAT metadata, the most popular metadata standard, defines the spatial extent of spatial datasets using bounding box coordinates or as links to gazetteers. Naive RAG is based on semantic similarity approaches.  An LLM can identify “Vienna” as a location, but would struggle to identify datasets relevant to the location, as there is little semantic similarity between the location name and coordinate digits or gazetteer links.  There is thus a need to incorporate spatial indexing techniques for improved spatial reasoning.

With our contribution we present an approach that combines LLMs, RAG, and spatial indexing techniques to overcome existing challenges in discovering spatial data in SDIs, and improve spatial data discovery through natural language queries.

How to cite: Ondieki, J. O., Rieke, M., and Jirka, S.: Using Large Language Models to Enhance Spatial Data Discovery in Spatial Data Infrastructures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20221, https://doi.org/10.5194/egusphere-egu26-20221, 2026.

The recent rise of foundation models in Earth Observation (EO) has reshaped how remote sensing tasks are approached, particularly by allowing strong downstream performance with comparatively limited labeled data. These models have reported impressive results in applications such as land cover classification and semantic segmentation. However, performance gains alone do not resolve a central concern: whether the resulting predictions can be trusted. In practical EO scenarios—including disaster response and environmental monitoring—miscalibrated confidence estimates may lead to incorrect decisions even when overall accuracy appears high.

Motivated by this gap between accuracy and reliability, this study focuses on the uncertainty calibration behaviour of fine-tuned EO foundation models. Using TorchGeo for consistent data handling and the Lightning-UQ-Box framework for uncertainty quantification, we construct an evaluation pipeline that contrasts Vision Transformer–based pretrained models with conventional convolutional neural networks trained from scratch. Experiments are conducted across both image classification tasks (e.g., EuroSAT) and dense prediction settings such as semantic segmentation.

Rather than assuming superior representations automatically yield better-calibrated predictions, we explicitly examine how calibration properties change after fine-tuning large pretrained models. In addition, we evaluate a spectrum of uncertainty quantification approaches, from lightweight post-hoc methods like temperature scaling to more computationally demanding techniques, including Monte Carlo Dropout, deep ensembles, and Laplace approximation. Calibration quality is assessed using expected calibration error and reliability diagrams, alongside predictive accuracy.

By analysing the trade-offs between computational cost, accuracy, and calibration, this work provides practical insight into which UQ strategies are most effective for EO foundation models. Our findings aim to support the deployment of remote sensing systems in operational settings where reliable uncertainty estimates are as critical as raw predictive performance.

How to cite: Wei, Y.: Uncertainty Quantification for Earth Observation Foundation Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20813, https://doi.org/10.5194/egusphere-egu26-20813, 2026.

Localized rapid urban expansion and global climate change have contributed to land use and land cover (LULC) dynamic modifications, which further links to changed land surface temperatures (LST). This study proposes an integrated approach of machine learning (ML) models in assessing decadal LULC changes and future prediction in a city in the Mekong region. To achieve an accurate LULC map object-based classification strategies were implemented using various ML techniques across observed years with four main land cover categories: built-up areas, water bodies, paddy fields/shrubs, and orchards, together with LST extraction. The findings reveal that Random Forest classifier works superior to other classifiers, achieving the best overall accuracy of 81%. There have been substantial land usage changes, with the percentage of developed areas rising from 8% in 2014 to approximately 12% in 2024. Urbanization is correlated with rising temperatures , while, vegetation, on the other hand, helps alleviate this heat by providing shade and cooling. With an overall accuracy of 85% in the patch-generating land use simulation (PLUS) model, by 2030, under the impacts of both natural and socio-economic drivers, an apparent increase in the proportion of built-up areas to 15% and a slight variation in other categories could be seen in line with planning objectives. The urban expansion could be clearly seen in the highly dense districts with an increase to 42% by 2030 from an initial stage of merely 27% in 2014. The primary forecast conversions in LULC observed were vegetated lands transforming into construction areas for urbanization, yet maintaining agricultural practices for food security. The integrated approach has proven its suitability in intricate land usage patterns evaluation and optimization.

How to cite: Nguyen, L. and Daou, D.: Harnessing an Integrated Machine Learning based Approach in Monitoring and Predicting Dynamic Spatiotemporal Land Use and Land Cover Changes. A case study in a Mekong city , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21002, https://doi.org/10.5194/egusphere-egu26-21002, 2026.

EGU26-21265 | PICO | ESSI1.7

Spatially-explicit uncertainty assessment of ecosystem extent mapping 

Polina Tregubova, Sylvie Clappe, Ida Marielle Mienna, Bruno Smets, Marcel Buchhorn, Ruben Remelgado, and Carsten Meyer

Ecosystems are a key component of biodiversity, providing vital services to humans and the economy. Anthropogenic pressures driving environmental change result in widespread ecosystem degradation and loss. The area and spatial distribution of ecosystem types, referred to as ecosystem extent, provide a critical entry point for assessing ecosystem condition, functioning, and associated services, and therefore require detailed and spatially explicit monitoring.

Despite advances in geospatial analysis, consistent mapping and delineation of ecosystem extent remain challenging. Map products on ecosystem extent should, therefore, be supported by uncertainty assessments, ideally in a spatially explicit manner. According to best practices in related fields, the minimum requirement for uncertainty quantification for thematic maps is the aggregated estimation of per-class accuracy and per-class area uncertainty, following a validation procedure based on independent reference data. However, the standard practice remains spatially implicit. To date, there is no established practice for spatially explicit uncertainty quantification procedures.

This study presents a spatial solution for estimating the uncertainty of maps produced using machine-learning algorithms. The approach builds on the standard map-validation procedure and extends it to pixel-wise assessments using conformal prediction. While conformal prediction can be applied to any machine learning algorithm, ecosystem extent mapping poses domain-specific challenges, including a high-dimensional multi-class setting and hierarchical class structures. This study, therefore, focuses on developing solutions to ensure robust class-specific coverage, exploring different conformal prediction implementation variants, and adapting them from flat to hierarchical mapping scenarios.

To assess the feasibility and applicability of our approach, we tested it on the Oslo-Viken municipality in Norway. In this case study, we developed an ecosystem extent map for 2024 and quantified and mapped its uncertainty at pixel-level. This analysis helped to evaluate the practical application and performance of the approach on real-world cases.

 

How to cite: Tregubova, P., Clappe, S., Marielle Mienna, I., Smets, B., Buchhorn, M., Remelgado, R., and Meyer, C.: Spatially-explicit uncertainty assessment of ecosystem extent mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21265, https://doi.org/10.5194/egusphere-egu26-21265, 2026.

EGU26-4 | ECS | Posters on site | HS6.5

Advanced phycocyanin detection in a South American lake using Landsat imagery and remote sensing 

Lien Rodríguez-López, David Bustos Usta, Lisandra Bravo Alvarez, Iongel Duran Llacer, Luc Bourrel, Frederic Frappart, and Roberto Urrutia

In this study, multispectral images were used to detect toxic blooms in Villarrica Lake in Chile, using a time series of water quality data from 1989 to 2024, based on the extraction of spectral information from Landsat 8 and 9 satellite imagery. To explore the predictive capacity of these variables, we constructed 255 multiple linear regression models using different combinations of spectral bands and indices as independent variables, with phycocyanin concentration as the dependent variable. The most effective model, selected through a stepwise regression procedure, incorporated seven statistically significant predictors (p < 0.05) and took the following form: FCA = N/G + NDVI + B + GNDVI + EVI + SABI + CCI. This model achieved a strong fit to the validation data, with an R2 of 0.85 and an RMSE of 0.10 μg/L, indicating high explanatory power and relatively low error in phycocyanin estimation. When applied to the complete weekly time series of satellite observations, the model successfully captured both seasonal dynamics and interannual variability in phycocyanin concentrations (R2 = 0.92; RMSE = 0.05 μg/L). These results demonstrate the robustness and practical utility for long-term monitoring of harmful algal blooms in Lake Villarrica.

How to cite: Rodríguez-López, L., Bustos Usta, D., Bravo Alvarez, L., Duran Llacer, I., Bourrel, L., Frappart, F., and Urrutia, R.: Advanced phycocyanin detection in a South American lake using Landsat imagery and remote sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4, https://doi.org/10.5194/egusphere-egu26-4, 2026.

EGU26-125 | ECS | Orals | HS6.5

Flood Dynamics and Frequency Mapping in the Lower Ganges Floodplain in India Using Multi-Temporal Sentinel-1 SAR Observations (2016–2024) 

Mohammad Sajid, Haris Hasan Khan, Arina Khan, and Abdul Ahad Ansari

The Ganges floodplains are among the most flood-prone regions in India, where recurrent inundations cause significant socio-economic and ecological impacts. Understanding the spatial distribution, frequency, and dynamics of flooding is essential for effective floodplain management and enhancing climate resilience. This study examines the flood frequency and spatial extent across a section of the Ganga River floodplains in Bihar, utilising multi-temporal Sentinel-1 Synthetic Aperture Radar (SAR) data spanning the period from 2016 to 2024. Flooded areas were delineated through an optimal threshold-based classification of VH-polarised backscatter images, with threshold values ranging from -19.5 dB to -22.3 dB. Annual flood extents were mapped, and an inundation frequency composite was generated to identify zones experiencing recurrent flooding. The spatial analysis revealed substantial variability in flood occurrence, with extensive inundation observed in low-lying regions. Several areas were inundated in more than 60% of the study years, indicating chronic flood exposure. The decadal analysis revealed that August and September were the peak months for flooding, with some areas remaining inundated for more than one month, which had an adverse impact on both human settlements and agricultural lands. Validation using optical satellite imagery from Sentinel-2 confirmed a 98% accuracy in the SAR-derived flood extent, reinforcing the reliability of the classification method. The temporal flood frequency analysis provides crucial insights into long-term flood dynamics and helps identify hydrologically sensitive zones. Overall, this study highlights the effectiveness of SAR-based monitoring in understanding floodplain behaviour under changing climatic and hydrological conditions, and supports improved flood hazard mapping, hydrodynamic model calibration, and sustainable flood risk management in the Ganges Basin and other monsoon-affected regions.

Keywords: Flood Inundation, Multi-Temporal, Time-Series, Flood Frequency, Sentinel-1 SAR, Ganges River

How to cite: Sajid, M., Hasan Khan, H., Khan, A., and Ansari, A. A.: Flood Dynamics and Frequency Mapping in the Lower Ganges Floodplain in India Using Multi-Temporal Sentinel-1 SAR Observations (2016–2024), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-125, https://doi.org/10.5194/egusphere-egu26-125, 2026.

Wetlands are very sensitive hydrological ecosystems that are essential for groundwater recharge, flood control, and biodiversity. Climate variability, changed river regimes, and unsustainable anthropogenic pressures are all posing new challenges to their stability. The current work evaluates the two-decade hydro-climatic dynamics of the Haiderpur Wetland (Ganga River, India) by merging optical (Landsat), radar (Sentinel-1), and gridded climate (ERA5, CHIRPS) datasets with GRACE-based groundwater anomalies. On the Google Earth Engine (GEE), processing of time-series Landsat (NDVI, NDWI, LST) and Sentinel-1 (SAR) data to monitor all-weather surface inundation and vegetation structure. To disentangle climatic and anthropogenic drivers, these remote sensing products are statistically correlated against ERA5-Land (Evapotranspiration) and CHIRPS (Precipitation) data, alongside GRACE groundwater anomalies. The findings demonstrated a considerable downward trend in pre-monsoon NDWI and wetland water distribution. This was accompanied by a significant increase in LST and an unexpected increase in NDVI. All-weather Sentinel-1 data validated the drying trend. On the other hand, 'greening' (as indicated by NDVI) in a drying environment suggests a structural shift from native wetland vegetation to more drought-tolerant or invasive terrestrial plants. The study assesses the capability of a multifaceted (optical-radar-climate) GEE strategy to quantify the individual contributions of climatic and anthropogenic factors, while also monitoring wetland development. Furthermore, these findings quantify the hydro-ecological vulnerability of major Ramsar wetlands and emphasize the vital need for coordinated water management to sustain ecosystems in the Ganga River Basin, with far-reaching implications for global wetland conservation.

Keywords: Hydrology, GRACE, Climate Change, SAR, NDVI, NDWI, LST

How to cite: Ansari, A. A., Hasan Khan, H., Khan, A., and Sajid, M.: Hydro-Ecological Vulnerability of  Ganga River Wetland (India): A Multi-Sensor Remote Sensing and GRACE-based Assessment of the Haiderpur Ramsar Site, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-147, https://doi.org/10.5194/egusphere-egu26-147, 2026.

Floods are the costliest and most frequently occurring natural disasters. One of the key factors in preventing and reducing losses is providing a reliable flood map. However, the uncertainty associated with either flood inundation model or data, specifically the Digital Elevation Model (DEM), may have adverse effects on the reliability of flood stage and inundation maps. Therefore, a systematic understanding of the uncertainty is necessary. In this study, an attempt is made to assess whether models are more susceptible to the uncertainties or the data itself. In order to do this, a SCIFRIM (Slope-corrected, Calibration-free, Iterative Flood Routing and Inundation Model) is employed, utilizing a list of DEM datasets to reconstruct the October 2024 Valencia flood event. The modelled flood extents were validated against those derived from multi-sensor remote sensing data. The Critical Success Index (CSI) was calculated to assess the agreement between observed and modelled flood extents, yielding values of 0.49 and 0.59 for October 30th and 31st, respectively, when combining SCIFRIM and Lidar-DEM. Additionally, a multi-model comparison has been performed between SCIFRIM and CaMa-Flood (Catchment-based Macro-scale Floodplain), HEC-RAS (Hydrologic Engineering Center's River Analysis System), and TUFLOW (Two-dimensional Unsteady FLOW), demonstrating its relevance in terms of outputs (flood extent and stage) and model runtime. The findings demonstrate that the proposed modeling framework offers a reliable approach for flood assessment. It has great potential to support rapid assessment and decision-making in data-scarce regions.

How to cite: Tripathi, G., Sarkar, E., and Biswal, B.: Evaluating Slope-corrected, Calibration-free, Iterative Flood Routing and Inundation Model (SCIFRIM)-based Flood Inundation against multi-satellite observation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-436, https://doi.org/10.5194/egusphere-egu26-436, 2026.

Floods are highly dynamic hazards whose spatial extent can change rapidly within hours. Timely and accurate monitoring is essential for early warning, emergency response, and post-disaster assessment. A major challenge in current Earth Observation (EO) based approaches is the difficulty of capturing the complete evolution of a flood event, including its maximum flood extent. This information is often missing due to temporal gaps in Synthetic Aperture Radar (SAR) acquisitions and cloud cover in optical imagery. Missing the peak extent limits the accuracy of impact assessments and poses challenges for applications such as parametric insurance, which depend on reliable measurements of flood magnitude. Although daily flood products exist, they are often based on large-scale multi-spectral sensors and struggle during persistent cloud cover as well as with resolution for smaller events, creating an urgent need for a more reliable method for daily flood estimation from higher-resolution SAR datasets. To address these challenges, we propose a novel deep learning framework that fuses EO-based coarse dynamic hydrometeorological data with static geospatial datasets to produce high-resolution daily flood extent maps. Our approach integrates static flood conditioning inputs, including elevation, Height Above Nearest Drainage, Urban Development Area, flow direction, Normalized Difference Vegetation Index, Normalized Difference Built-up Index, soil clay and sand content, and pre-flood SAR and multispectral imagery with dynamic hydrometeorological variables such as daily precipitation and soil moisture. The model adopts a multi-stage vision transformer architecture: encoders extract multi-level latent representations from all inputs, which are then fused using cosine similarity, normalization, and temporal attention mechanisms. A decoder reconstructs high-resolution flood extent, followed by a Gaussian filter to reduce high-frequency noise. The framework is fully supervised using the globally available KuroSiwo flood mask dataset, ensuring transferability across diverse geographic regions and climate zones. In addition, this research provides a complete data preparation workflow that converts flood mask shapefiles into standardized image patch datasets, including a modular input selection interface that removes dependence on inputs included in specific datasets, directly suitable for deep learning training, enabling straightforward implementation and practical applicability. The model is trained and evaluated across three distinct climate zones on multiple continents, demonstrating a robust capability to overcome the temporal limitations of SAR data and cloud-induced gaps in optical observations. Held-out region tests with strict geographic separation to minimize spatial autocorrelation induced data leakage, further ensure unbiased evaluation and true transferability. Preliminary tests across multiple continents yield stable performance, with cross-site metric variations remaining within approximately 5-7 percent. This study introduces the first deep learning framework for daily fine-scale flood extent mapping using purely EO data which are globally accessible, providing a scalable and transferable solution for real-time flood monitoring, disaster management, and potential applications in parametric insurance by improving flood mapping cadence and reliably estimating maximum flood extents.

Keywords: spatio-temporal fusion, vision transformer, high-resolution flood mapping

How to cite: Surojaya, A., Kumar, R., and Dasgupta, A.: DeepFuse2.0: Novel Deep Learning-based Fusion of Satellite-based Hydroclimatic Data and Flood Conditioning Factors for Daily Flood Extent Mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1047, https://doi.org/10.5194/egusphere-egu26-1047, 2026.

EGU26-1092 | ECS | Posters on site | HS6.5

Cross-Biome Transferability of SAR-based Flood Mapping with Random Forests 

Paul Christian Hosch and Antara Dasgupta

Fully automated, globally applicable flood-mapping systems must earn user trust, which in turn requires systematic testing across diverse environmental conditions to understand performance stability and a clear understanding of model transferability. While some recent studies have evaluated cross-site performance of flood mapping algorithms, the cross-biome transferability of Random Forest (RF) models for SAR-based flood delineation has not yet been thoroughly evaluated. In this study, we assess how well RF classifiers trained for binary flood detection generalize across biomes using primarily Synthetic Aperture Radar (SAR) data. Our feature stack comprises 14 variables, including 9 SAR-derived features (Sentinel-1 VV and VH backscatter and associated temporal-change metrics) which provide information on the flood-induced land surface changes and 4 contextual predictors such as land cover and topographic indices which influence radar backscatter and help to reduce as well as mitigate uncertainties. Experiments were conducted across 18 flood events distributed equally amongst 6 distinct biomes: (1) Deserts and Xeric Shrublands, (2) Tropical and Subtropical Moist Broadleaf Forests, (3) Temperate Broadleaf and Mixed Forests, (4) Temperate Coniferous Forests, (5) Mediterranean Forests, Woodlands and Scrub, (6) Temperate Grasslands, Savannas and Shrublands. Model transferability is evaluated using a two-level nested cross-validation approach. First, intra-biome performance is established through an inner 3-fold Leave-One-Group-Out Cross-Validation (LOGO-CV), in which models are trained on all but one site within a biome and evaluated on the held-out site iteratively. Second, inter-biome transferability is quantified using an outer 6-fold LOGO-CV, treating each biome as a distinct group. In this setup, models are trained on all biomes except one and evaluated on all sites of the held-out biome. Classification performance is assessed using Overall Accuracy (OA), F1-score, Precision, Recall, and Intersection over Union (IoU), with all experiments repeated across 10 independent iterations to capture model structural and sampling variability.

Preliminary results on select biomes show substantial variation in inter-biome transferability. Notably, in some cases, models transferred between biomes outperform those trained within the same biome. These findings highlight the need for comprehensive biome-level transferability assessments to better understand the capabilities and limitations of RF-based flood mapping under globally diverse conditions, ultimately supporting more transparent and trustworthy flood-mapping products for end users.

How to cite: Hosch, P. C. and Dasgupta, A.: Cross-Biome Transferability of SAR-based Flood Mapping with Random Forests, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1092, https://doi.org/10.5194/egusphere-egu26-1092, 2026.

EGU26-1266 | ECS | Posters on site | HS6.5

Cross-Biome Feature Importance Stability Analysis for SAR-based Flood Mapping with Random Forests 

Parisa Havakhor, Paul Hosch, and Antara Dasgupta

Flood mapping using machine learning methods such as Random Forests (RF) requires informed feature engineering and selection. Despite feature-importance rankings across different biomes and land covers varying substantially, the stability of these feature rankings has not been evaluated specifically for RF-based flood delineation. In this study, we investigate the consistency of RF feature-importance rankings in a binary flood-classification task primarily based on Synthetic Aperture Radar (SAR) imagery. The feature stack comprises 14 variables, including 9 SAR-based features, Sentinel-1 VV and VH polarizations and their temporal-change metrics which inform the flood extent identification, and 4 contextual features such as land cover and topographic indices which provide information on backscatter uncertainties. The classification task was conducted across 18 flood events spanning six distinct biomes: (1) Deserts and Xeric Shrublands, (2) Tropical and Subtropical Moist Broadleaf Forests, (3) Temperate Broadleaf and Mixed Forests, (4) Temperate Coniferous Forests, (5) Mediterranean Forests, Woodlands and Scrub, and (6) Temperate Grasslands, Savannas and Shrublands. Three feature-attribution methods were evaluated: (1) Shapley Additive exPlanations (SHAP) provides a game-theoretic framework for feature attribution and is widely recognized for its consistency and interpretability; (2) Mean Decrease in Impurity (MDI), computed during tree growth, is the most commonly used importance metric for RF models; (3) Permutation feature importance (MDA) offers a model-agnostic approach that assesses importance by measuring the reduction in model accuracy when feature values are randomly shuffled. Both feature cardinality and feature correlation, which bias the feature rankings for these algorithms in different ways, were considered during interpretation. All experiments were repeated across 10 independent iterations to account for random variability. We first examined feature-importance rankings independently across the three sub-sample studies within each biome to establish baseline intra-biome variability, followed by quantification of inter-biome variability to assess whether feature-importance patterns transfer across different environmental conditions. Preliminary results across select biomes indicate stable rankings for SAR-based features, with VV and VH event polarizations dominating the decision boundary, while contextual descriptors, particularly terrain indices such as Height Above the Nearest Drainage, exhibit greater variability both within and between biomes. Understanding the transferability of feature-importance patterns and feature stacks across biomes is critical for developing an RF-based flood-mapping pipeline that operates reliably under diverse environmental conditions worldwide and ultimately builds user trust in the resulting products.

How to cite: Havakhor, P., Hosch, P., and Dasgupta, A.: Cross-Biome Feature Importance Stability Analysis for SAR-based Flood Mapping with Random Forests, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1266, https://doi.org/10.5194/egusphere-egu26-1266, 2026.

EGU26-1859 | ECS | Posters on site | HS6.5

Detecting Waterlogging in Agricultural Fields in Denmark using High-Resolution PlanetScope Time Series 

Jasper Kleinsmann, Julian Koch, Stéphanie Horion, Gyula Mate Kovacs, and Simon Stisen

Waterlogging in agricultural fields is the condition of temporally inundated areas driven by extreme rainfall, rising groundwater or poor drainage, and has been identified as a major issue by Danish farmers. During the inundation period, plants are deprived of oxygen which negatively affects the root development and leads to decreased yields and grain quality. Additionally, these waterlogged areas are a large source of greenhouse gas (GHG) emissions. The issue is expected to exacerbate under current climate projections through wetter winters and rising groundwater levels in Denmark. Hence, an increased understanding of the spatio-temporal dynamics of waterlogging is required to future-proof the management strategies. The research goals are three-fold: (1) to optimise the detection of waterlogging, (2) to reveal inter- and intra-annual patters across Denmark and (3) to investigate the drivers of waterlogging such as climate, topography and bio-physical conditions. We aim to detect waterlogged areas through a deep learning semantic segmentation approach utilising multi-temporal PlanetScope imagery and nation-wide high resolution elevation data. This approach requires a manually delineated reference dataset to train, validate and test the model which needs to be well-balanced spatially, e.g. covering various soil types, and temporally, e.g. including various illumination conditions. Additionally, we will experiment with various model architectures, backbones and covariate combinations to optimise the segmentation performance. Initial tests using a UNET architecture and building upon a published reference dataset by Elberling et al. (2023), show promising results and lay the foundation for the upcoming model development and extension of the existing reference data.

 

Elberling, B. B., Kovacs, G. M., Hansen, H. F. E., Fensholt, R., Ambus, P., Tong, X., ... & Oehmcke, S. (2023). High nitrous oxide emissions from temporary flooded depressions within croplands. Communications Earth & Environment, 4(1), 463.

 

How to cite: Kleinsmann, J., Koch, J., Horion, S., Kovacs, G. M., and Stisen, S.: Detecting Waterlogging in Agricultural Fields in Denmark using High-Resolution PlanetScope Time Series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1859, https://doi.org/10.5194/egusphere-egu26-1859, 2026.

EGU26-2995 | ECS | Orals | HS6.5

SaferSat: The Saferplaces’s  Operational Sentinel-1 Toolbox for Multi-Temporal Flood Extent Mapping, Water-Depth Estimation and Impact Assessment  

Saeid DaliriSusefi, Paolo Mazzoli, Valerio Luzzi, Francesca Renzi, Tommaso Redaelli, Marco Renzi, and Stefano Bagli

Operational flood intelligence for emergency response and insurance, providing a rapid overview of impacted land, population, and economic damages, requires mapping solutions that remain reliable under adverse observational conditions and across diverse landscapes. Although Sentinel-1 SAR provides consistent global, all-weather and day-and-night coverage, automated flood extraction is challenged by speckle noise, land-cover heterogeneity, and confusion between floodwater and permanent low-backscatter surfaces. These limitations highlight the need for approaches that exploit temporal backscatter changes while maintaining global robustness and computational efficiency.

We present SaferSat, a fully automated Sentinel-1 toolbox for flood-extent mapping, water-depth estimation, and impact assessment. SaferSat is part of SaferPlaces (saferplaces.co), a global Digital Twin platform for flood risk intelligence supporting emergency response and insurance applications. Central to the framework is Pr-RWU-Net (Progressive Residual Wave U-Net), a lightweight deep-learning model with 2.6 million trainable parameters, designed to detect flood-induced backscatter changes using VV-polarized SAR imagery. The model uses a three-channel input; pre-event VV, post-event VV, and their radiometric difference, enhancing inundation sensitivity while mitigating VH instability for global deployment.

SaferSat provides end-to-end processing: automated data retrieval, multi-date flood inference, and Maximum Flood Extent generation. To reduce SAR ambiguities, it generates auxiliary layers: a vegetation mask for SAR "blind spots" and a low-backscatter anomaly mask for permanent dark features. Flood extent layers are integrated with the FLEXTH model and GLO-30 or local high-resolution LiDAR DTMs for water-depth reconstruction. The system also analyzes acquisition patterns to predict short-term revisit opportunities. Impact assessment intersects flood extents with JRC GHS-POP and ESA WorldCover datasets.

The Pr-RWU-Net model was trained on the S1GFloods dataset, containing 5,360 paired pre- and post-event Sentinel-1 GRD images across 42 flood events from 2016–2022. Binary flood masks were generated via semi-automated thresholding and expert quality control. Evaluation on the test split achieved an IoU of 90.0%, F1-score 94.6%, Recall 95.6%, Precision 93.8%, and overall accuracy 96.6%.

Operational applicability was demonstrated on three 2025 flood events: Romania, Pakistan, and France. SaferSat flood extents closely matched SAR manual driven flood references (IoU 89–92%) and CEMS products (IoU 85–88%). Water-depth estimation against a reference hydrodynamic model yielded a MAE of 34–40 cm and correlation R of 0.78–0.82. For a 260 km² flood in Romania, the full processing chain completed in ~3 minutes on a standard CPU, demonstrating suitability for rapid, large-scale deployment.

SaferSat is available globally through SaferPlaces, supporting emergency response and insurance applications. Future developments aim to enhance SaferSat globally via integration of commercial satellite data to reduce revisit time and rapid hydrodynamic modeling to address radar limitations.

How to cite: DaliriSusefi, S., Mazzoli, P., Luzzi, V., Renzi, F., Redaelli, T., Renzi, M., and Bagli, S.: SaferSat: The Saferplaces’s  Operational Sentinel-1 Toolbox for Multi-Temporal Flood Extent Mapping, Water-Depth Estimation and Impact Assessment , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2995, https://doi.org/10.5194/egusphere-egu26-2995, 2026.

EGU26-3018 | Posters on site | HS6.5

Advancing Flood Forecasting in Large River Basins Using Multi-Mission Satellite Data: the EO4FLOOD project 

Angelica Tarpanelli and the EO4FLOOD Team

Floods are among the most destructive natural hazards worldwide, causing severe impacts on human health, ecosystems, cultural heritage and economies. Over the past decades, both developed and developing regions have experienced increasing flood-related losses, a trend that is expected to intensify under climate change due to shifts in precipitation patterns and the frequency of extreme events. In many large river basins, particularly in data-scarce regions, flood forecasting remains highly uncertain because of limited in situ observations and complex hydrological and hydraulic dynamics.

EO4FLOOD is an ESA-funded project aimed at demonstrating the added value of advanced Earth Observation (EO) data for improving flood forecasting at regional to continental scales. The project focuses on the integration of multi-mission satellite observations with hydrological and hydrodynamic modelling frameworks to support flood prediction up to seven days in advance, with an explicit treatment of uncertainty.

A key outcome of EO4FLOOD is the development of a comprehensive and openly available EO-based dataset designed to support flood modelling and forecasting studies. The dataset covers nine large and hydrologically complex river basins worldwide, selected to represent a wide range of climatic, physiographic and anthropogenic conditions, and characterized by limited or heterogeneous availability of ground-based observations. It integrates high-resolution satellite products from ESA and non-ESA missions, including precipitation, soil moisture, snow variables, flood extent, water levels and satellite-derived river discharge.

Within EO4FLOOD, these EO datasets are combined with hydrological and hydraulic models, enhanced by machine learning techniques, to improve flood prediction skill and to better quantify predictive uncertainty in data-scarce environments. The project also investigates the role of human interventions, such as reservoirs and land-use changes, in modulating flood dynamics across the selected basins.By making this multi-variable EO dataset publicly available, EO4FLOOD aims to support the broader hydrological community in testing, benchmarking and developing flood modelling and forecasting approaches in challenging large-basin settings. The project provides a unique opportunity to explore the potential and limitations of EO-driven flood forecasting and contributes to advancing the use of satellite observations for global flood risk assessment and management.

How to cite: Tarpanelli, A. and the EO4FLOOD Team: Advancing Flood Forecasting in Large River Basins Using Multi-Mission Satellite Data: the EO4FLOOD project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3018, https://doi.org/10.5194/egusphere-egu26-3018, 2026.

            Water security in the Chi River Basin is critical for the agricultural economy and ecosystem stability of Yasothon Province, Thailand. However, effective spatiotemporal monitoring of water surface dynamics is frequently hindered by persistent cloud cover during the monsoon season, limiting the utility of traditional optical remote sensing. This study addresses this challenge by developing a robust Multi-Sensor Deep Learning Fusion system that integrates Synthetic Aperture Radar (SAR) and optical satellite imagery to ensure continuous observation capabilities.

            We employ a U-Net convolutional neural network architecture, selected for its high boundary precision and efficiency with limited training datasets. The model is trained on a fused six-channel input configuration, combining Sentinel-1 SAR data (weather-independent) with Sentinel-2 optical bands (RGB), augmented by the Normalized Difference Water Index (NDWI) and Normalized Difference Vegetation Index (NDVI). This multi-modal approach enhances feature extraction, allowing for the accurate differentiation of open water from floating vegetation and flooded agricultural lands in complex transition zones.

            The study analyzes the hydrological cycle of 2022, capturing distinct drought, flood, and post-flood conditions. To ensure hydrological validity, the model’s segmentation outputs are not merely visually assessed but are quantitatively validated against ground-truth water level data from the E.20A gauge station in Kham Khuean Kaeo District. By establishing a precise Stage-Area Relationship, this research demonstrates a scalable, cost-effective framework for flood risk assessment and water capital estimation, offering a resilient solution for river basin management in cloud-prone tropical regions.

How to cite: Pruekthikanee, P.: Multi-Sensor Deep Learning Fusion for Spatiotemporal Water Surface Monitoring in the Yasothon Province's Chi River Basin, Thailand, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4154, https://doi.org/10.5194/egusphere-egu26-4154, 2026.

EGU26-5752 | ECS | Orals | HS6.5

Satellite-Enhanced Flood Modelling for the Niger River Basin using a Synergy of Hydrological Modelling and Earth Observation Data 

Shima Azimi, Alexandra Murray, Connor Chewning, Cecile Kittel, Henrik Madsen, Fan Yang, Maike Schumacher, and Ehsan Forootan

Accurate water cycle representation in data-scarce and flood-prone regions like the Niger River Basin demands stronger integration between remote sensing and hydrological modelling. Spanning ten water-stressed nations, this basin faces critical challenges under climate change, requiring robust water-budget assessments to guide resilience strategies. We employ DHI’s Global Hydrological Model (DHI-GHM) to simulate key hydrological components of the regional water cycle. Model outputs for surface and root-zone soil moisture (SSM and R-ZSM) and terrestrial water storage (TWS) are systematically compared against satellite observations (GRACE/GRACE-FO and multiple soil moisture products) to identify discrepancies and enhance the understanding of regional hydrological behavior. A near real-time SSM data assimilation scheme is implemented to enhance spatiotemporal accuracy of surface and top-soil interactions, particularly beneficial in the flood-sensitive Inner Niger Delta. Post-assimilation hydrological outputs are coupled with the CaMa-Flood surface hydraulic model to simulate inundation dynamics, enabling improved flood prediction and supporting risk management. Finally, we pursue two-way coupling of hydrological and hydrodynamic models by integrating river flow–storage feedbacks to advance flood forecasting and sustainable water-resources planning. 

How to cite: Azimi, S., Murray, A., Chewning, C., Kittel, C., Madsen, H., Yang, F., Schumacher, M., and Forootan, E.: Satellite-Enhanced Flood Modelling for the Niger River Basin using a Synergy of Hydrological Modelling and Earth Observation Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5752, https://doi.org/10.5194/egusphere-egu26-5752, 2026.

EGU26-5862 | ECS | Orals | HS6.5

Refining global wetland characterization using an unsupervised, wetness-based dynamic framework 

Yang Li, Nandin-Erdene Tsendbazar, Kirsten de Beurs, Lassi Päkkilä, and Lammert Kooistra

Existing global wetland datasets and monitoring approaches emphasizepersistent inundation, while intermittent inundation and waterlogged states—especially where vegetation is present—are underrepresented or of lower accuracy. This leads to inaccurate estimates of greenhouse gas emissions from carbon-rich systems (e.g., peatlands). Meanwhile, the predominance of annual mapping limits the capture of intra-annual variability, further reinforcing these inaccuracies and obscuring sub-seasonal disturbances from human activities (e.g., shifts in rice-cropping intensity). This study presents an unsupervised, wetness-driven framework for improving global wetland monitoring that leverages earth observation data streams. For framework development, the OPtical TRApezoid Model is applied to Harmonized Landsat-Sentinel imagery to retrieve surface wetness, followed by wetland delineation using a scene-adaptive grid-based thresholding algorithm. This framework is applied to 824 globally distributed 0.1° grid cells encompassing 9,781 land-cover-labeled sites and 134 sites with daily wet–dry labels across 28 Ramsar wetlands, and validated for spatial delineation, thematic, and temporal accuracy. Comparative analysis employs Dynamic World, the first global 30 m wetland map with a fine classification system (GWL_FCS30), and the modified Dynamic Surface Water Extent algorithm (DSWE). Our framework achieved moderate spatial delineation accuracy with F1 of 0.64 (recall 0.75, precision 0.56), comparable in F1 to Dynamic World and with higher recall than DSWE and GWL_FCS30. It delivered the highest temporal accuracy (F1 0.72; precision 0.81; recall 0.64) and improved thematic accuracy for vegetated wetland, reducing omission with modest commission. The proposed wetland monitoring framework enables more accurate targeted policy interventions.

How to cite: Li, Y., Tsendbazar, N.-E., de Beurs, K., Päkkilä, L., and Kooistra, L.: Refining global wetland characterization using an unsupervised, wetness-based dynamic framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5862, https://doi.org/10.5194/egusphere-egu26-5862, 2026.

EGU26-6114 | ECS | Orals | HS6.5

Evidential Deep Learning for Uncertainty-Aware Global Flood Extent Segmentation 

Chi-ju Chen and Li-Pen Wang

Flood extent mapping from satellite imagery plays a critical role in disaster response and flood risk management, particularly as flood events become more frequent and severe under a changing climate. At its core, the task involves classifying each pixel in an optical satellite image as flooded or non-flooded. Recent deep learning-based segmentation models have demonstrated strong performance at the global scale. However, despite their accuracy, most existing approaches provide deterministic predictions and offer limited information on the reliability of individual pixel-level outputs. This lack of uncertainty information constrains their operational applicability, especially in high-risk scenarios where models may exhibit overconfident but incorrect predictions.

To address this limitation, we extend a global flood extent segmentation framework by explicitly incorporating uncertainty quantification. Specifically, an Evidential Deep Learning (EDL) approach is integrated into a UNet++ architecture within the ml4floods framework, enabling simultaneous prediction of flood extent and associated pixel-wise uncertainty. Within the EDL formulation, network outputs are interpreted as evidence and parameterised using a Beta distribution, providing a principled estimate of predictive uncertainty. Furthermore, total uncertainty is decomposed into aleatoric and epistemic components, allowing clearer interpretation of whether uncertainty arises from data ambiguity or from limited model knowledge.

The proposed approach is evaluated using the extended WorldFloods global flood dataset. Preliminary results indicate that the EDL-enhanced model maintains promising segmentation performance while producing informative uncertainty maps. Elevated uncertainty is consistently observed in misclassified regions and along land-water boundaries, where optical signals are inherently ambiguous. These results demonstrate that uncertainty estimates offer valuable insight into model reliability and support operational decision-making by highlighting areas that require closer inspection. In practice, uncertainty-guided triage can help prioritise expert review and resource allocation, focusing attention on regions where decision risk is highest.

How to cite: Chen, C. and Wang, L.-P.: Evidential Deep Learning for Uncertainty-Aware Global Flood Extent Segmentation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6114, https://doi.org/10.5194/egusphere-egu26-6114, 2026.

EGU26-6180 | ECS | Orals | HS6.5

 The capabilities of virtual gauging stations in satellite monitoring of water bodies 

Ildar Mukhamedjanov and Gulomjon Umirzakov

Remote sensing technologies provide effective tools for monitoring and assessing the state of inland water bodies, enabling extraction of various hydrological parameters from satellite observation. Central Asian and some African countries are currently implementing practical programs aimed at mitigating water scarcity and improving the management of transboundary water resources. Rivers and their tributaries flowing across national boundaries require continuous monitoring to support early warning of droughts and floods at the basin scale.

Conventional ground-based hydrological stations are traditionally used to measure water level, estimate daily river discharge, and support hydrological forecasting. However, limitations related to accessibility, data-sharing restrictions, and the high cost of installation and maintenance often constrain their spatial coverage and long-term operation.  Virtual gauging station (VGS) represents a complementary remote-sensing approach, providing time series derived from the long-term satellite image archives. A VGS is defined as a free-shaped polygon on the map used to analyze data within the borders of this polygon and collect observations based on the requirements. Currently, VGS applications primarily rely on optical satellite imagery from Sentinel-2, Landsat-4, -5, -7, -8, -9 missions to estimate water surface area (WSA) using spectral water index (MNDWI, AWEI or AWEIsh). Variations in WSA serves as a proxy for surface water availability and river dynamics. 

In addition, VGS can be used to enrich satellite altimetry-based water level (H) time series. For this purpose, the VGS polygon is calibrated using reference altimetric observations obtained from open-access data source (e.g. SDSS, DAHITI, Hydroweb). Calibration involves estimating the parameters of a regression model describing the functional relationship between water level and water surface area.  The resulting values can finally be integrated into hydrological models to support short-term river discharge forecasting. Thus, VGS provides continuous hydrological information independent of ground-based measurements, while optional validation against in-situ observations allows for the assessment of the model uncertainty.  Based on the experimental analysis, optimal placement of VGS polygons is recommended dynamically active river sections that account for annual riverbed displacement, as well as in river reaches located near satellite altimeter ground tracks to improve calibration accuracy.

The experiments demonstrated that correlation between ground truth and forecasted water level values is upper 0,85 and mean absolute error is lower than 0,3 m. The following result has been obtained using linear regression which shows that application of more complex forecasting models could significantly improve the results.

How to cite: Mukhamedjanov, I. and Umirzakov, G.:  The capabilities of virtual gauging stations in satellite monitoring of water bodies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6180, https://doi.org/10.5194/egusphere-egu26-6180, 2026.

EGU26-6408 | ECS | Posters on site | HS6.5

Multisensor Ensemble Mapping of Sub-hectare Ephemeral Surface Water in Kenyan ASALs 

James Muthoka, Pedram Rowhani, Chloe Hopling, Omid Memarian Sorkhabi, and Martin Todd

Ephemeral pans and seasonal ponds in arid and semi-arid lands supply critical water for pastoral and ecological systems, yet are not routinely monitored due to their small size, highly dynamic and spectral confusion with vegetation and shadows. We present and evaluate a multisensor mapping approach to detect sub-0.5 ha surface water bodies and quantify their linkage to rainfall variability to inform decision making.

Our approach fuses Sentinel-1 SAR, Sentinel-2 optical indices and DEM derived covariates within an ensemble classifier (voting of Random Forest, Gradient Boosting, and Decision Tree models). Predictive uncertainty is mapped using ensemble agreement and class probabilities, and we compare SAR-only, optical-only, terrain-only, and fused configurations. Additionally, rain and ephemeral surface water dynamics are modelled using generalised additive models with CHIRPs  and local rain gauge observations to test the lagged relationships in monthly water area anomalies.

Results show the fused model achieves an overall accuracy of 85%, outperforming Sentinel-1, and Sentinel-2 (78% and 72%, respectively). Generalised additive models explain 62% of variance in monthly water area anomalies, with a strong response at 1-3 month lags. These results show multisensor fusion with  quantified uncertainty improves detection of ephemeral surface water and enables estimation of rainfall thresholds and lagged dynamics relevant to pastoral water planning and targeted anticipatory action interventions.

How to cite: Muthoka, J., Rowhani, P., Hopling, C., Memarian Sorkhabi, O., and Todd, M.: Multisensor Ensemble Mapping of Sub-hectare Ephemeral Surface Water in Kenyan ASALs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6408, https://doi.org/10.5194/egusphere-egu26-6408, 2026.

EGU26-6586 | ECS | Posters on site | HS6.5

Do Geospatial Foundation Models Improve SAR-Based Flood Mapping?  

Antara Dasgupta and Moetez Zouaidi

Accurate and timely flood delineation is a cornerstone of disaster response and hydrological risk management. Synthetic Aperture Radar (SAR) is uniquely suited to this task because it operates independently of cloud cover and illumination, yet its interpretation remains challenging due to speckle, terrain effects, vegetation scattering, and ambiguities between flooded and permanent water as well as shadows and smooth surfaces such as tarmac. While deep learning has substantially advanced SAR-based flood segmentation, most existing models are trained from scratch and often struggle to generalize across regions and flood regimes. Recently, geospatial foundation models (GFMs) pretrained on massive satellite archives have shown promise, but their benefits for SAR-based flood mapping remain insufficiently quantified. This paper presents a controlled, large-scale global scale evaluation and benchmarking of a vision-transformer based GFM (NASA IBM Prithvi) against two task-specific segmentation architectures, the SegFormer (hierarchical transformer) and the commonly used U-Net (convolutional neural network), including lightweight variants, for post-event SAR-based flood mapping. All models were trained and evaluated under a standardized pipeline that explicitly addresses extreme class imbalance via stratified negative sampling and weighted loss functions. Training and validation used the expert-annotated Kuro Siwo dataset (43 flood events, 67,490 Sentinel-1 VV/VH tiles), while generalization is assessed on both the in-distribution Kuro Siwo test set and the out-of-distribution Sen1Floods11 hand labelled benchmark dataset. Results show that stratified negative sampling (controlling how many background-only tiles are shown to the model in each training epoch) increases precision by approximately 6% and mean Intersection-over-Union (mIoU) by about 7% relative to no sampling, while stabilizing training loss dynamics. On the in-distribution data, all architectures reach similar performance (mIoU ≈ 0.82), indicating that well-designed task-specific models remain competitive with GFMs. However, under out-of-distribution conditions, the foundation model Prithvi (mIoU 0.768) closely matches the performance of the SegFormer (mIoU 0.772) and clearly outperforms the U-Net (mIoU 0.712), highlighting the robustness of transformer-based representations when transferring across datasets. Pretraining on optical imagery yields only modest gains for SAR (+3.4% mIoU), suggesting that architectural inductive biases and data handling matter more than cross-modal pretraining. Notably, lightweight GFM variants achieve comparable accuracy with up to 94% fewer parameters, demonstrating strong potential for operational deployment. Scene-level analysis reveals that CNNs suppress scattered false alarms due to the neighborhood contextualization but miss large, continuous floods, while transformers preserve spatial coherence yet overpredict along complex boundaries and scattered surface water ponding, especially near permanent water bodies. Findings demonstrate that while SAR-based flood mapping accuracy requires a combination of appropriate model architectures and class imbalance-aware training, rather than foundation-scale pretraining alone. However, for spatial and statistical transfer to out of distribution datasets, GFMs offer substantial advantages and provide above-average performance for unseen cases, even without localized fine-tuning.

How to cite: Dasgupta, A. and Zouaidi, M.: Do Geospatial Foundation Models Improve SAR-Based Flood Mapping? , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6586, https://doi.org/10.5194/egusphere-egu26-6586, 2026.

EGU26-6617 | ECS | Posters on site | HS6.5

SARFlood: A Web-Based, Cloud-Native Platform for Automated and Optimized ML-based SAR Flood Mapping    

Patrick Wilhelm, Paul Hosch, and Antara Dasgupta

Synthetic Aperture Radar (SAR) imagery offers weather-independent observation capabilities critical for monitoring flood events. However, SAR-based flood detection workflows typically require specialized software, local computational resources, and expert knowledge in remote sensing. This work presents SARFlood, a web-accessible application that automates the complete SAR flood detection pipeline using the OpenEO platform. SARFlood is built on a Flask backend architecture designed for accessibility and reproducibility. Users interact with the system through a web interface that guides them through case study creation, including Area of Interest (AOI) definition via shapefile upload, event date specification, and optional ground truth data integration. The application implements OpenEO OAuth 2.0 authentication using the device code flow, enabling secure access to the Copernicus Data Space Ecosystem (CDSE) backend without requiring users to manage API credentials locally. Session-based project management allows users to track processing progress in real-time through a status reporting system that monitors each pipeline stage. Data acquisition is performed server-side via OpenEO, while feature engineering processors execute locally. The data acquisition module fetches multiple data sources through a unified OpenEO interface: pre-event and post-event Sentinel-1 VV and VH imagery, Digital Elevation Models (DEM) with automatic source fallback (FABDEM, Copernicus 30m/90m), and ESA WorldCover land cover classification. The OpenStreetMap water body features and the FathomDEM are acquired via their own APIs/websites. A caching system prevents redundant API calls for previously acquired datasets, significantly reducing processing time for iterative analyses, while keeping licensing in mind so only users who are logged in and have the according license will be able to access the cached files. The processing pipeline computes a comprehensive feature stack for flood detection. SAR derivatives include intensity bands, VV/VH polarization ratios, and change detection metrics computed in decibel space to enhance flood signal discrimination. Topographic features encompass slope and Height Above Nearest Drainage (HAND) derived from the DEM, as key indicators of flood susceptibility. Flow direction calculations use an expanded bounding box to determine the extended HAND computation domain to address edge artifacts, finally cropped to the original AOI during band compilation, ensuring computationally efficient and accurate flow routing. Additionally, stream burning is implemented to improve drainage network delineation. Further, contextual features include Euclidean Distance to Water and rasterized land cover classification. Users can currently upload ground truth shapefiles (e.g., Copernicus EMS), which are automatically rasterized and compiled into the output stack, enabling supervised classification workflows.  

SARFlood includes integrated sampling and training modules. Multiple strategies such as Simple Random, Stratified, Generalized Random Tessellation Stratified, and Systematic Grid sampling are supported. The training module implements Random Forest classification with Leave-One-Group-Out Cross-Validation across multiple case studies, hyperparameter optimization via Bayesian search, and feature importance assessment through Mean Decrease Impurity, permutation importance, and SHAP values. The platform-, data- and model-agnostic design principles used in developing SARFlood, support open science and FAIR practices in the geoscience community. By combining web accessibility with robust feature engineering and machine learning integration, SARFlood provides researchers with a reproducible platform for generating uncertainty-aware flood labels lowering barriers to use. 

How to cite: Wilhelm, P., Hosch, P., and Dasgupta, A.: SARFlood: A Web-Based, Cloud-Native Platform for Automated and Optimized ML-based SAR Flood Mapping   , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6617, https://doi.org/10.5194/egusphere-egu26-6617, 2026.

EGU26-7132 | ECS | Orals | HS6.5

Monitoring Freshwater Bodies over the Past 40 Years Using Synthetic Monthly Sentinel-2 MSI Imagery  

Federica Vanzani, Patrice Carbonneau, Simone Bizzi, Martina Cecchetto, and Elisa Bozzolan

In the last decade rapid advancements in remote sensing have opened new frontiers in our ability to monitor freshwater bodies dynamics at the global scale. Most works have taken advantage of the long time series of Landsat constellations (30 m resolution) relying on spectral indices to identify water. Recently, much progress has also been made in the development and use of deep learning models capable of explicit semantic classification of river water, lake water and sediment bars, based on Sentinel-2 (S2) MSI imagery (10 m resolution). In this work, we present an approach that seeks to extend these existing, trained, fluvial landscape classification models to Landsat data in order to observe long-term water and morphological shifts in rivers and lakes. Rather than explicitly re-training the models with Landsat data and labour-intensive manual label data, we apply a domain transfer approach to generate synthetic S2 MSI imagery from Landsat inputs. This approach has the advantage that the training of deep learning domain transfer models only requires synchronous Landsat and Sentinel data and thus obviates the need for manual labels.

The results show that, when using these synthetic images, river water, lake water and sediment bars are classified with an F1 score of 0.8, 0.94, 0.65 respectively, which represents a decrease of ca. 10% for river water and 20% for sediment with respect to real S2 imagery. By adopting this integrated approach, we are therefore able to monitor, for the first time, lake water, river water and sediment bars at 10 m resolution, over a 40-year period, integrating both synthetic S2 and real S2 acquisitions through a single, fluvial landscape segmentation model. Classification obtained from median monthly images can then be aggregated at the yearly or multi-yearly scale to delineate river or lake water fluctuations, and active channels (river water plus sediment bars) trajectories, from specific freshwater bodies to the global scale.

How to cite: Vanzani, F., Carbonneau, P., Bizzi, S., Cecchetto, M., and Bozzolan, E.: Monitoring Freshwater Bodies over the Past 40 Years Using Synthetic Monthly Sentinel-2 MSI Imagery , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7132, https://doi.org/10.5194/egusphere-egu26-7132, 2026.

EGU26-7320 | ECS | Posters on site | HS6.5

Evaluating multimodal optical and SAR learning strategies for flood and surface water delineation 

jiayin xiao, zixi li, and fuqiang tian

Flood and surface water mapping from satellite observations remains challenging due to the complementary yet heterogeneous characteristics
of optical and synthetic aperture radar (SAR) data. While deep learning has achieved promising results, existing studies are often evaluated on
isolated datasets or focus on a single modality, limiting their comparability and operational relevance. In this study, we conduct a large-scale and systematic evaluation of optical, SAR, and combined optical–SAR learning strategies for flood and surface water mapping across multiple public satellite benchmarks. Using a common training and evaluation protocol, we compare lightweight convolutional networks and large pretrained vision models under single-modality and multimodal settings. The analysis reveals that attention-based multimodal fusion consistently improves water delineation accuracy on most datasets, while model capacity and preprocessing choices play a critical role in balancing missed detections and false alarms. On global-scale benchmarks, moderately sized backbones coupled with dedicated fusion mechanisms achieve robust performance without relying on extremely large models.These findings provide practical guidance for selecting architectures and fusion strategies in operational flood mapping and establish a reproducible benchmark for future optical and SAR studies.

How to cite: xiao, J., li, Z., and tian, F.: Evaluating multimodal optical and SAR learning strategies for flood and surface water delineation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7320, https://doi.org/10.5194/egusphere-egu26-7320, 2026.

EGU26-7998 | Orals | HS6.5

Ten years of floods across Europe mapped from space with reconstructed water depths  

Andrea Betterle and Peter Salamon

Floods are among the most deadly and destructive natural disasters. Improving our understanding of large-scale flood dynamics is crucial to mitigating their dramatic consequences. Unfortunately, systematic observation-based datasets—especially featuring flood depths—have been lacking.

This contribution presents advancements in developing an unprecedented catalogue of satellite-derived flood maps across Europe from 2015 onwards. Results are based on the systematic identification of floods in the entire Sentinel-1 archive at 20 m spatial resolution as provided by the Global Flood Monitoring component of the Copernicus Emergency Management Service. Using a novel algorithm that accounts for terrain topography, flood maps are enhanced and provided with water depth estimates—a critically important information for flood impact assessments.

The resulting dataset represents a significant step towards the creation of a global flood archive. It provides new tools for interpreting flood hazards on large scales, with substantial implications for flood risk reduction, urban development planning, and emergency response.

How to cite: Betterle, A. and Salamon, P.: Ten years of floods across Europe mapped from space with reconstructed water depths , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7998, https://doi.org/10.5194/egusphere-egu26-7998, 2026.

EGU26-8292 | Posters on site | HS6.5

Modelling wetland resilience to climate change and anthropogenic impacts. 

Patricia Saco, Rodriguez Jose, Breda Angelo, Eric Sandi, and Steven Sandi

Coastal wetlands provide a wide range of ecosystem services, including shoreline protection, attenuation of storm surges and floods, water quality improvement, wildlife habitat and biodiversity conservation. These ecosystems have been observed to sequester atmospheric carbon dioxide at rates significantly higher than many other ecosystems, positioning them as promising nature-based solutions for climate change mitigation.  However, projections of coastal wetland conditions under sea-level rise (SLR) remain highly variable, owing to uncertainties in environmental factors as well as the necessary simplifications embedded within the wetland evolution modelling frameworks. Assessing wetland resilience to rising sea levels and the effect of anthropogenic activities is inherently complex, given the uncertain nature of key processes and external influences. To enable long-term simulations that span extensive temporal and spatial scales, models must rely on a range of assumptions and simplifications—some of which may significantly affect the interpretation of wetland resilience.

 

Here we present a novel eco-hydro-geomorphological modelling framework to predict wetland evolution under SLR. We explore how accretion and lateral migration processes influence the response of coastal wetlands to SLR, using a computational framework that integrates detailed hydrodynamic and sediment transport processes. This framework captures the interactions between physical processes, vegetation, and landscape dynamics, while remaining computationally efficient enough to support simulations over extended timeframes. We examine several common simplifications employed in models of coastal wetland evolution and attempt to quantify their influence on model outputs. We focus on simplifications related to hydrodynamics, sediment transport, and vegetation dynamics, particularly in terms of process representation, interactions between processes, and spatial and temporal discretisation. Special attention is given to identifying modelling approaches that strike a balance between computational efficiency and acceptable levels of accuracy. We will present recent model results to assess the resilience of coastal wetland to SLR on several sites around the world and will discuss new results to assess the effect of human interventions and infrastructure on wetland resilience.

How to cite: Saco, P., Jose, R., Angelo, B., Sandi, E., and Sandi, S.: Modelling wetland resilience to climate change and anthropogenic impacts., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8292, https://doi.org/10.5194/egusphere-egu26-8292, 2026.

EGU26-9354 | ECS | Orals | HS6.5

L-band InSAR to complement SAR inundation mapping under vegetation 

Clara Hübinger, Etienne Fluet-Chouinard, Daniel Escobar, and Fernando Jaramillo

Wetland inundation dynamics are key for understanding flood regulation, ecosystem functioning and greenhouse gas emissions. Synthetic Aperture Radar (SAR) can map water extent independent of cloud cover and can partly penetrate vegetation, particularly at L-band. Many SAR inundation products rely primarily on intensity thresholding and indicators such as specular reflection and double-bounce scattering. However, these approaches can underestimate inundation extent in densely vegetated wetlands where volume scattering can obscure the water signal. Here we demonstrate how L-band interferometric SAR (InSAR) can complement intensity-based inundation mapping under vegetation by exploiting phase differences between repeat SAR acquisitions. Using ALOS PALSAR-1 and PALSAR-2, together providing a nearly two-decade observational archive, we show that L-band InSAR can capture inundation dynamics in tropical floodplain wetlands, such as the Atrato floodplain (Colombia) and Amazon várzea floodplains (e.g., along the Río Pastaza). In the Atrato floodplain, the InSAR-derived flooded vegetation extent shows pronounced seasonal variability, ranging from ~500 to >1500 km² during 2007–2011. Comparison with existing L-band SAR inundation products yields ~70% overall agreement, while InSAR consistently detects broader inundated extents in densely vegetated floodplain areas where intensity-based thresholding underestimates inundation. This complementarity among methodologies is particularly relevant for inundation extent data products from the NASA–ISRO NISAR mission, which are expected to rely largely on SAR backscatter thresholding. Our results highlight the value of integrating InSAR-derived information to strengthen wetland inundation monitoring under vegetated canopies.

How to cite: Hübinger, C., Fluet-Chouinard, E., Escobar, D., and Jaramillo, F.: L-band InSAR to complement SAR inundation mapping under vegetation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9354, https://doi.org/10.5194/egusphere-egu26-9354, 2026.

EGU26-9758 | ECS | Orals | HS6.5

Hydrologically-Informed DTM Super-Resolution for Rapid Flood Depth Estimation 

Sandro Groth, Marc Wieland, Christian Geiß, and Sandro Martinis
Reliable estimation of flood depths from satellite-derived inundation extent information critically depends on the spatial resolution and hydrological consistency of the underlying digital terrain model (DTM). Accurate, very high–resolution DTMs are typically not publicly available, difficult to access within the time constraints of rapid mapping, and lack consistent coverage. Although open-access DTMs such as the Forest and Buildings removed Copernicus DEM (FABDEM) provide global coverage, their coarse spatial resolution often fails to represent important small-scale terrain features that control flow paths, slopes, and local water accumulation. To address these limitations, this study proposes a deep learning framework for DTM super-resolution that combines low-resolution DTMs with optical satellite imagery by integrating hydrological knowledge into the training process to force the reconstruction of relevant topographic features for improved flood inundation depth estimation.

The proposed approach employs a residual channel attention network (RCAN) enhanced with optical satellite imagery as auxiliary input to upscale low-resolution terrain data. Central to the methodology is a collaborative hydrologic loss function that guides network optimization beyond elevation-based accuracy. In addition to the mean absolute elevation error (MAE), the loss integrates slope deviation and flow direction disagreement to focus the learning on the reconstruction of terrain features that are directly relevant for hydrologic applications.

Unlike other super-resolution approaches, which are often using downscaled versions of the low-resolution inputs to learn super-resolved DTMs, the proposed framework was trained on a growing set of aligned patches of real-world globally available low-resolution elevation data, optical satellite imagery, and high-resolution reference DTMs derived from airborne LiDAR. Model performance is evaluated against conventional interpolation and standard super-resolution baseline architectures, including convolutional neural networks (CNN) as well as geospatial foundation models (GFM). To assess the practical impact on flood mapping, the super-resolved DTMs are tested on a set of real-world flood events in Germany by using the well-known Flood Extent Enhancement and Water Depth Estimation Tool (FLEXTH) to derive inundation depth metrics.

Results show that integrating DTMs derived using hydrologically guided super-resolution into flood depth tools can lead to more accurate flood depth estimates compared to low-resolution or other super-resolved inputs. The added hydrologic loss significantly improves the preservation of slopes and flow directions while maintaining elevation accuracy.

Overall, the presented framework offers a method to generate hydrologically meaningful high-resolution DTMs from globally available low-resolution inputs to benefit flood depth estimation in areas, where no high-resolution terrain information is available.

How to cite: Groth, S., Wieland, M., Geiß, C., and Martinis, S.: Hydrologically-Informed DTM Super-Resolution for Rapid Flood Depth Estimation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9758, https://doi.org/10.5194/egusphere-egu26-9758, 2026.

Flash flood disasters have increased by more than 50% in the first 20 years of the 21st century compared to the last 20 years of the 20th century. Monitoring and understanding flood events might lead to better mitigation of this natural hazard. Using SAR and SAR interferometry (InSAR) proved to be a useful tool for mapping flooded areas due to the lower backscatter or decorrelation of the SAR signal in an open-water environment. In Arid regiem, flash flood water is rapidly drained by evaporation or percolation, often before the satellite image is acquired. To overcome this challenge, we propose in this study to use the InSAR coherency loss, created by surface changes during a flash-flood, to map the runoff path and utilize it to quantify peak discharge (Qmax).

We focus on the Ze’elim alluvial fan along the western shore of the Dead Sea, Israel, an arid area affected by seasonal flash floods a few days a year. We use 34 interferograms of X-band (COSMO-SkyMed/TerraSAR-X) SAR data, covering 25 runoff events between 2017 and 2021, and upstream hydrological gauge data. To consider the natural decorrelation processes, we calculate a normalized coherence (ϒn) term, using the average coherence of the study area and the average coherence of a stable reference area, identified by differential LiDAR measurements.

We find a strong correlation between gn and the logarithm of the peak discharge (Qmax). However, the method is limited by a minimal peak discharge—where energy is too low to change the surface—and maximal total water volume—where decorrelation is saturated. The method may provide tools for reconstructing runoff data in arid areas where historical SAR data is available, and for monitoring in difficult access areas or where hydrological stations are sparse or damaged.

How to cite: Nof, R.: Estimating Flash Flood Discharge in Arid Environments Using InSAR Coherence: A Case Study of the Ze’elim Fan, Dead Sea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11948, https://doi.org/10.5194/egusphere-egu26-11948, 2026.

EGU26-12249 | Orals | HS6.5 | Highlight

Lessons Learned from Remote Sensing of River Ice for Flood Early Warning 

Arjen Haag, Tycho Bovenschen, Elena Vandebroek, Athanasios Tsiokanos, Ben Balk, and Joost van der Sanden

Rivers in regions with cold winters can seasonally freeze up. River ice breakup and freeze-up processes can lead to river ice jams, which are a major contributor to flood risk in cold regions (across most of the high latitudes of the northern hemisphere). In Canada, satellite remote sensing is used across the country to provide timely information on the status of river ice. Methods and algorithms to classify various stages of river ice from the Radarsat Constellation Mission (RCM) are available, but the operational implementation of these, especially the integration into larger flood forecasting and early warning systems, requires specific expertise, software and computational resources, and comes with its own set of challenges. In collaboration with various agencies across Canada we have set up operational monitoring systems with the purpose of assisting the daily tasks of forecasters on duty. These have been used in practice over multiple ice breakup and freeze-up seasons, which has highlighted both their usefulness and shortcomings. We will focus on various aspects of such a system and share lessons learned on its design, setup and operational use, as well as a framework to analyse various factors relevant for operational monitoring purposes (e.g. spatiotemporal coverage and latency of the data, critical elements in the support of decision-making relating to floods). In this, we do not shy away from problems and pitfalls, so that others can learn from these. While various challenges remain, this work is a good example of the value in the joint engagement of applied science and end users.

How to cite: Haag, A., Bovenschen, T., Vandebroek, E., Tsiokanos, A., Balk, B., and van der Sanden, J.: Lessons Learned from Remote Sensing of River Ice for Flood Early Warning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12249, https://doi.org/10.5194/egusphere-egu26-12249, 2026.

EGU26-13343 | Posters on site | HS6.5

Operational, national-scale monitoring of river trajectories using satellite imagery  

Elisa Bozzolan, Marco Micotti, Elisa Matteligh, Alessandro Piovesan, Federica Vanzani, Patrice Carbonneau, and Simone Bizzi

The global degradation of river ecosystems and the growing impacts of flood hazards have highlighted limitations in current river management approaches. In Europe, the Water Framework and Flood Directives promote integrated, catchment-scale assessments of hydromorphological conditions and flood risk. Such integration is essential for sustainable management. Planform dynamics and river bed aggradation/incision, for example, can modify channel conveyance and compromise flood mitigation measures, whereas granting more space to rivers can both enhance ecological quality and reduce flood peaks.

In this context, the availability of long-term satellite archives and advances in computational and machine-learning methods enable large-scale, high spatiotemporal resolution monitoring of large and medium river systems. However, despite this potential, the operational adoption of satellite-based river monitoring remains limited due to data complexity, interdisciplinary requirements, and the lack of harmonised computational infrastructures.

Thanks to a collaboration between industry, public institutions and the university, we developed a methodology to systematically map monthly water channel, channel width, sediment bars and vegetation dynamics, testing the results on the full archive of Sentinel-2 (10 m resolution) for medium-large Italian rivers (active channel > 30m - i.e. 3 Sentinel-2 pixels). In this talk, I will outline the applied methodology, discuss its applicability at national scale with Sentinel-2 data, and show how the generated products can better inform river habitat mapping, river conservation practices, and flood risk assessments by supporting consistent national scale geomorphic trajectories identification.

How to cite: Bozzolan, E., Micotti, M., Matteligh, E., Piovesan, A., Vanzani, F., Carbonneau, P., and Bizzi, S.: Operational, national-scale monitoring of river trajectories using satellite imagery , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13343, https://doi.org/10.5194/egusphere-egu26-13343, 2026.

Flood inundation mapping has become increasingly critical as climate change intensifies the frequency and severity of flooding worldwide, amplifying risks to populations, infrastructure, and ecosystems. Recent advances in Earth Observation (EO) have shown unprecedented opportunities to monitor flood dynamics across large spatial scales.. However, significant challenges remain due to the limitations of single-sensor approaches. While multispectral imagery provides rich semantic information, it is frequently constrained by cloud cover during flood events. Conversely, Synthetic Aperture Radar (SAR) offers all-weather capability but suffers from signal ambiguity in complex terrains and urban environments. Effectively integrating these heterogeneous modalities therefore remains a challenge, particularly with limited labelled flood event data.

In this study, we propose a deep learning-based cross-modal fusion framework that leverages the representational capacity of Remote Sensing Foundation Models (RSFMs). High-level feature embeddings are extracted from Sentinel-1 and Sentinel-2 multispectral imagery by initializing modality-specific encoders with pretrained weights from state-of-the art multi-modal foundation models, providing a robust and semantically aligned feature space despite limited task-specific training data 

To integrate the multi-modal representations, we adopt a Gated Cross-Modal Attention mechanism, which adaptively modulates the information flow from each modality based on their observation reliability. Specifically, the model is trained to prioritise SAR features to ensure spatial continuity under cloud-obscured conditions, while simultaneously leveraging richer optical semantics to disambiguate SAR signals, correcting for example false detections caused by radar shadowing or smooth impervious surfaces. 

To assess the generalisation of the proposed framework across diverse regions and sensor conditions, we trained and evaluated our model using a comprehensive dataset compiled from publicly available benchmarks, including Kuro Siwo and WorldFloods. Our framework not only establishes a new benchmark for all-weather flood monitoring but also demonstrates the critical role of remote sensing foundation models in overcoming the limitations of traditional, data-hungry fusion approaches.

How to cite: Chen, Y. C. and Wang, L. P.: Integrating SAR and Multispectral Satellite Observations for Flood Inundation Mapping: A Cross-Modal Fusion Framework Leveraging Foundation Models and Gated Attention Mechanism, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13502, https://doi.org/10.5194/egusphere-egu26-13502, 2026.

EGU26-13888 | ECS | Posters on site | HS6.5

A Comparative Assessment of Threshold-Based and Machine Learning Methods for Flood Detection 

Jawad Mones, Saeed Mhanna, Landon Halloran, and Philip Brunner

 

Flood mapping plays a key role in understanding hazard impacts, supporting emergency response, and guiding long-term risk planning. Remote sensing is now widely used in flood studies because it offers low-cost data, avoids the need for dangerous field surveys, and provides rapid observations over large areas. Despite these advantages, comparative research remains limited, particularly with respect to differences among flood-mapping algorithms, such as machine-learning versus threshold-based approaches, and the performance of optical versus radar sensors. This research addresses these gaps by applying multiple flood-mapping methods to the same flood event in Pakistan, and then comparing their performance with respect to a validation benchmark to provide a clearer insight into how data selection and methodological design influence flood detection outcomes

This study evaluates four distinct methods for mapping floods using multi-sensor satellite data. To ensure a fair comparison, three unsupervised machine-learning approaches including a synergetic Sentinel-1 and Sentinel-2 workflow, a method integrating harmonized Landsat–Sentinel data with radar, and a daily MODIS imagery technique were tested alongside a traditional Otsu thresholding baseline. All four were tested on the same 2025 Pakistan flood event, characterized by intense monsoon rains and flash flooding across regions such as Sindh and Punjab in mid- to late-2025.  The flood maps were then validated against UNOSAT flood reports for this event, where UNOSAT’s flood extent closely matches the results produced by the Sentinel-1/Sentinel-2 workflow, which yields the most conservative flood extent among the tested methods.

 Larger flood extents from some methods, especially the Sentinel-1 Otsu thresholding approach, include areas not clearly flooded in optical images. This happens because SAR backscatter also responds to wet soil and saturated vegetation, which a simple threshold can misclassify as water, leading to flood overestimation.

Overall, the results show that flood maps are not just different versions of the same answer, they reflect different satellite data and the utilized algorithms detect flooding. Approaches that combine multiple data sources with machine-learning strike a better balance, producing flood extents that are both spatially consistent and physically realistic. This indicates that multi-sensor, machine-learning–based methods are better suited for operational flood monitoring than simple thresholding, which is too sensitive to surface noise and often overestimates flooding. 

How to cite: Mones, J., Mhanna, S., Halloran, L., and Brunner, P.: A Comparative Assessment of Threshold-Based and Machine Learning Methods for Flood Detection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13888, https://doi.org/10.5194/egusphere-egu26-13888, 2026.

EGU26-16468 | ECS | Orals | HS6.5

Multidecadal Changes and Trends in Global River Positions 

Elad Dente, John Gardner, Theodore Langhorst, and Xiao Yang

Rivers play a central role in shaping the Earth's surface and ecosystems through physical, chemical, and biological interactions. The intensity and locations of these interactions change as rivers continuously migrate across the landscape. In recent decades, human activity and climate change have altered river hydrology and sediment fluxes, leading to changes in river position, or migration. However, a comprehensive perspective on and understanding of these recent changes in the rate of river position shifts is lacking. To address this knowledge gap, we created a continuous global dataset of yearly river positions and migration rates over the past four decades and analyzed trends. The global annual river positions were detected using Landsat-derived surface water datasets and processed in Google Earth Engine, a cloud-based parallel computation platform. The resulting river extents and centerlines reflect the yearly permanent position, corresponding to the rivers’ location during base flow. This approach improves the representation of position changes derived from geomorphological rather than hydrological processes. To robustly analyze river position changes across different patterns and complexities and at large scales, we developed and applied a global reach-based quantification method.

Results show that while alluvial rivers maintain stable positions in certain regions, others exhibit trends in the rates of position change. For instance, the Amazon Basin, which has experienced significant deforestation and hydrological modifications, has shown increased rates of river position change in recent decades, directly modifying active floodplains. In this presentation, we will discuss the advantages, limitations, and applications of the global yearly river position dataset, offer insights into the changing rates of river position, and highlight current and future impacts on one of Earth’s most vulnerable hydrologic systems.

How to cite: Dente, E., Gardner, J., Langhorst, T., and Yang, X.: Multidecadal Changes and Trends in Global River Positions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16468, https://doi.org/10.5194/egusphere-egu26-16468, 2026.

Satellite-based surface water monitoring is essential for traking the spatiotemporal dynamics of global water bodies. However, most existing systems rely on a single mission or sensor modality, constraining both accuracy and temporal coverage. To overcome these limitations, we propose a multi-mission data fusion framework that integrates SAR Sentinel-1 and optical Sentinel-2 observations. Two U-Net convolutional neural networks were trained independently on the S1S2-Water dataset: one using Sentinel-1 sigma-nought backscatter (VV/VH) and the other using Sentinel-2 RGB and NIR bands, with terrain slope incorporated as ancillary input in both models. Predictive uncertainty is quantified via Monte Carlo dropout embedded within the networks, modeling pixel-wise predictions as Gaussian distributions. These probabilistic outputs are subsequently fused using a Bayesian framework and refined through sensor-specific exclusion masks. Evaluation across 16 geographically diverse test sites demonstrates that the fused probabilistic predictions achieve an overall IoU of 89%, highlighting the synergistic benefits of uncertainty-aware, multi-sensor integration. Furthermore, we show that model evaluation restricted to cloud-free optical imagery introduces substantial bias, limiting applicability for near-real-time monitoring. The proposed framework improves temporal availability, robustness, and reliability, advancing multi-satellite approaches for global surface water monitoring.

How to cite: Hassaan, M., Festa, D., and Wagner, W.: SAR and optical imagery for dynamic global surface water monitoring: addressing sensor-specific uncertainty for data fusion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17524, https://doi.org/10.5194/egusphere-egu26-17524, 2026.

EGU26-18308 | Orals | HS6.5

RESCUE_SAT project: Leveraging Satellite Data to Improve Large‑Scale Flood Modeling 

Elena Volpi, Stefano Cipollini, Luciano Pavesi, Valerio Gagliardi, Richard Mwangi, Giorgia Sanvitale, Irene Pomarico, Aldo Fiori, Deodato Tapete, Maria Virelli, Alessandro Ursi, and Andrea Benedetto

The RESCUE_SAT project was launched as part of the “Innovation for Downstream Preparation for Science” (I4DP_SCIENCE) programme (Agreement no. 2025‑2‑HB.0), funded by the Italian Space Agency (ASI), with the goal of enhancing the performance of the RESCUE model through the integration of satellite data. RESCUE is a large‑scale inundation model that enables probabilistic flood‑hazard assessment over large areas by preserving computational efficiency while explicitly representing hydrologic-hydraulic processes along the full drainage network. Primarily based on digital terrain models (DTMs), RESCUE is a hybrid framework that combines a geomorphology-based representation of the river network with simplified hydrological and hydraulic formulations to estimate water levels and inundation extents. The central challenge of the RESCUE_SAT project is to deliver a flood‑modelling tool capable of providing a more reliable and detailed representation of both large‑scale hydrological behavior and local hydraulic processes, including flow interactions with structures such as levees, bridges and dams which are currently not explicitly represented in RESCUE. To this purpose, the Synthetic Aperture Radar (SAR) imagery acquired by the ASI’s COSMO-SkyMed constellation is processed using interferometric techniques to derive high-resolution digital elevation models (DEMs), reaching meter-scale resolution. Starting from high-resolution DEMs derived from COSMO-SkyMed satellite imagery, RESCUE_SAT enables the identification of the locations of structures that interacts with flow propagation, supporting their systematic mapping. Once the infrastructures have been identified and parameterized from the high-resolution DEM, the DEM is resampled and processed to a computationally advantageous coarser resolution, while the detected infrastructure elements are directly integrated into the hydrological–hydraulic model.

How to cite: Volpi, E., Cipollini, S., Pavesi, L., Gagliardi, V., Mwangi, R., Sanvitale, G., Pomarico, I., Fiori, A., Tapete, D., Virelli, M., Ursi, A., and Benedetto, A.: RESCUE_SAT project: Leveraging Satellite Data to Improve Large‑Scale Flood Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18308, https://doi.org/10.5194/egusphere-egu26-18308, 2026.

EGU26-18518 | Orals | HS6.5

Automated Detection of Flood Events from CYGNSS: Observing Flood Evolution Along Propagating Tropical Waves  

Zofia Bałdysz, Dariusz B. Baranowski, Piotr J. Flatau, Maria K. Flatau, and Clara Chew

Flooding is a major natural hazard across the global tropics. Although flood occurrence is shaped by rainfall characteristics—including duration, frequency, and intensity—accurate prediction remains challenging. A key limitation is the lack of reliable, long-term flood databases that capture events across all spatial scales and durations, hindering a clear understanding of how rainfall variability translates into flood onset. This limitation is particularly critical in the Maritime Continent, where extreme rainfall is common and many small, short-lived, yet severe, floods remain undocumented. To address this limitation, we investigate whether a relatively new approach, global navigation satellite system reflectometry (GNSS-R), can help close this observational gap.

In this work, we assess whether data from the CYGNSS small-satellite constellation can be used to identify small- to regional-scale floods, including short-lived events. Our study focuses on Sumatra, an island within the Maritime Continent that is frequently affected by such hazards. A joint analysis of CYGNSS inundation estimates and two independent flood databases allowed us to evaluate how CYGNSS measurements can be used for flood detection. Three detailed case studies demonstrate that CYGNSS provides an unprecedented ability to monitor day-to-day changes in surface water extent, including floods at the urban scale. Specifically, we show that CYGNSS-derived inundation anomalies can clearly capture evolution of a flooding event, with the largest signature one day after known flood initiation. A systematic analysis of 555 flood events over a 21-month period enabled us to identify characteristic patterns in inundation anomalies that reliably distinguish flood events from non-flooding conditions, through the definition of an inundation-anomaly threshold and a maximum distance between CYGNSS detections and reported flood locations. We established that CYGNSS observations within 15 km not-only significantly differ from base-line conditions, but they allow tracking day-to-day flood dynamics as well.

The proposed methodology is transferable and can be applied to establish flood-inundation thresholds for any region within the global tropics, enabling automated detection of previously unreported flood events or the study of relationships between extreme precipitation and flood evolution. An example of its application is the automatic detection of flooding from CYGNSS data associated with subseasonal variability in tropical circulation: the passage of multiple convectively coupled Kelvin waves embedded within an active Madden–Julian Oscillation in July 2021. These waves propagated eastward across the Maritime Continent, triggering extreme rainfall and widespread flooding in equatorial Indonesia and East Malaysia. The day-to-day evolution of floods could be observed alongside the propagating waves, with the termination of the MJO coinciding with the cessation of the flood events.

Relying on low-cost small satellites, this approach shows strong potential for future scalability with larger constellations, ultimately improving flood monitoring and advancing our understanding of how rainfall patterns shape flood dynamics across global tropics.

How to cite: Bałdysz, Z., Baranowski, D. B., Flatau, P. J., Flatau, M. K., and Chew, C.: Automated Detection of Flood Events from CYGNSS: Observing Flood Evolution Along Propagating Tropical Waves , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18518, https://doi.org/10.5194/egusphere-egu26-18518, 2026.

Accurate long-term monitoring of surface water dynamics in the Niger River and Lake Chad basins is crucial for regional ecological security and sustainable water resource management. However, such monitoring is often hindered by insufficient continuous high-frequency observations—necessary to capture rapid shifts between permanent and seasonal water bodies in semi-arid transition zones—as well as by persistent cloud cover. To address these limitations, we developed a spatio-temporal data fusion framework designed to delineate detailed evolutionary patterns and regime shifts in surface water. Our methodology integrates Sentinel-1 SAR, Sentinel-2 optical imagery, and digital elevation model (DEM) data, adopting a “zoning modeling” strategy to reduce sensor-specific biases and environmental noise, thereby producing annual and seasonal surface water distribution maps. Furthermore, we developed a pixel-level, climate-coupled model based on inundation frequency to quantify changes in the extent, timing, and type of water bodies across a multi-year time series. Integration of these outputs elucidated the spatial heterogeneity of water resources throughout the study region from 2015 to 2024. Validation using randomly distributed reference samples demonstrated strong consistency, with overall accuracy exceeding 90%, confirming the robustness of our framework. Through an ecology-oriented classification scheme, we identified permanent water bodies—largely concentrated in the southern reaches of the Niger River main channel and the central zone of Lake Chad—as serving a “core support” function within the ecosystem. In contrast, seasonal water bodies followed a “dense in the south, sparse in the north” spatial pattern and acted as critical “ecological buffers” for arid northern areas. Notably, seasonal water extent expanded significantly during high-rainfall years such as 2018 and 2022, underscoring its pronounced sensitivity to climatic variability. Compared with current state-of-the-art approaches, the proposed framework enables characterization of high-frequency surface water dynamics and associated ecological interactions as continuous spatio-temporal fields, thereby providing a reliable and scalable tool to inform sustainable watershed management strategies across Africa.

How to cite: Du, L., You, S., Ye, F., and He, Y.: Tracking Dynamic Regimes and Ecological Functions of Surface Water in the Niger-Lake Chad Basins through Multi-Source Fusion (2015–2024), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19055, https://doi.org/10.5194/egusphere-egu26-19055, 2026.

EGU26-19963 | ECS | Orals | HS6.5

Development of routine flood mapping using SAR satellite observation for long-term monitoring system in the flood-prone regions, Cambodia 

Chhenglang Heng, Vannak Ann, Thibault Catry, Vincent Herbreteau, Cyprien Alexandre, and Renaud Hostache

Monitoring inland surface water in near-real time is a key challenge in cloud-prone tropical regions.  Recently, Synthetic Aperture Radar (SAR) products have been widely used to detect surface water. Our area of interest, the Tonle Sap Lake region is a complex environment where very large areas and floodplains are partially or fully submerged seasonally. As the population living around the lake strongly rely on the seasonal flooding dynamics for their socio-economic activities and can at the same time be at risk due to extreme flooding events, it is of main importance to develop tools for the monitoring of flooded areas. In this context, we are adopting and evaluating an algorithm which relies on parametric thresholding, and region growing approaches applied over time series of Sentinel-1 (S1) SAR backscatter images (VV and VH). To evaluate the produced water extent maps based on VV and VH polarizations, we used a cross evaluation using multi-sensor products: high-resolution optical data such as Sentinel-2 (S2) and the coarser resolution Sakamoto flood extend derived from MODIS product. The comparison is made using the Critical Success Index (CSI) and Kappa coefficient performance metrics. During the dry season, the VV polarization demonstrated very good performance using S2-derived maps as a reference, with CSI of 0.84 and a Kappa coefficient of 0.91, indicating highly accurate surface water detection. Performance was similar using the Sakamoto product as a reference (CSI=0.87). However, performance dropped during the rainy season, with the VV polarization's CSI decreasing to 0.76 comparing S2, reflecting challenges in detecting water in the extensive flooded vegetation areas. VH polarization consistently overestimated water extent by misclassifying wet vegetation and rice fields. A merge of VV and VH product yielded an intermediate performance, improving water detection in vegetated areas compared to VV alone. This comprehensive, multi-sensor and multi-season assessment clarifies the specific strengths of each S1 polarization, showing VV's superiority for open water mapping, especially in the dry season. It underscores the importance of selecting the appropriate product (VV for open water, merged for total inundation) and considering seasonal context for operational monitoring, thereby demonstrating the algorithm's robustness while also defining its operational limitations.

How to cite: Heng, C., Ann, V., Catry, T., Herbreteau, V., Alexandre, C., and Hostache, R.: Development of routine flood mapping using SAR satellite observation for long-term monitoring system in the flood-prone regions, Cambodia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19963, https://doi.org/10.5194/egusphere-egu26-19963, 2026.

The research focused on developing the framework for assessing marine, nearshore and transitional waters across Ireland and validated for generalization of the framework across at any geospatial scale using remote sensing (RS) products. To the best of authors knowledge, existing most of the studies only have demonstrated for retrieving particular water quality (WQ) indicators like turbidity, salinity or chlorophyll a without in depth validation results. Recently the authors comprehensively reviewed several studies focusing on the RS applications for assessing WQ using computational intelligence techniques (CIT) like machine learning, artificial intelligence, statistical approaches etc. Unfortunately, the reviewed findings reveals that most of the research are questionable in terms of using data transparency, and validation with independent or other geospatial domains applications of the existing developed tools. Therefore, the research aim was to develop a novel framework and validated with independent datasets including new domain(s) adaptation or validation. For developing the framework, to achieve the goal of the research, the study utilized Sentinel-3 (S3) OLCI RS reflectance data. For obtaining RS data, the study utilized S3-OLCI level 3(L3) and level 4 (L4) reflectance data Rhow_1 to Rhow_11 form the Copernicus Marine Services (CMS) repository datasets for 2016 to 2024. To obtain the overall WQ, the research considered 49 (in-situ) EPA, Ireland monitoring sites across various transitional and coastal waterbodies for computing the overall WQ (IEWQI scores) scores using recently developed and widely validated the IEWQI model. After than the RS data prepared and match-up with 49 considering monitoring sites. For predicting IEWQI scores, the research utilized the multi-scale signal processing framework (MSSPF) by following configurations: data augmentations: 2x to 20x, noise level from 0.0001 to 0.05, and data spilled ratios 60-20-20 and 70-20-10, respectively for train, test and validation of 43 CIT models using RS data from 2016 to 2023 both L3 and L4, whereas the 2024 dataset using for testing independent dataset to generalize the model prediction capabilities. Utilizing four identical model performance evaluation metrics, the results reveals that the PyTorchMLP could be effective (train performance : R2 = 0.86, RMSE =0.09, MSE = 0.008, and MAE = 0.067; test performance : R2 = 0.84, RMSE =0.094, MSE = 0.008, and MAE = 0.071; and validation performance : R2 = 0.81, RMSE =0.095, MSE = 0.009, and MAE = 0.074, respectively at 7x augmentation with 0.0001 of noise level for 60-20-20) compared to the 43 CIT models in terms of predicting and validating independent dataset (independent dataset validation performance for 2024 : R2 = 0.62, RMSE =0.164, MSE = 0.026, and MAE = 0.12). Based on the predicted IEWQI scores, the WQ ranked “marginal”, “fair” and “good” categories for Irish waterbodies. The findings of the framework align with the traditional EPA, Ireland monitoring approaches. However, findings of the research reveals that the proposed framework could be effective to monitoring WQ general purposes using RS data across any geospatial resolution.

Keywords: remote sensing; Copernicus database; MSSPF, IEWQI, Ireland.

How to cite: Uddin, M. G., Diganta, M. T. M., Sajib, A. M., Rahman, A., and Indiana, O.: A comprehensive framework for assessing marine, nearshore and transitional waters quality integrating Irish Water quality Index (IEWQI) model from remote sensing products using computational intelligence techniques, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20016, https://doi.org/10.5194/egusphere-egu26-20016, 2026.

EGU26-20097 | ECS | Orals | HS6.5

Comprehensive validation of the benefits of multi-sensor flood monitoring 

Chloe Campo, Paolo Tamagnone, Guy Schumann, Trinh Duc Tran, Suelynn Choy, and Yuriy Kuleshov

Multi-sensor methodologies are gaining traction within flood monitoring research, grounded in the rationale that data fusion from diverse sources mitigates uncertainty and improves spatiotemporal coverage. However, these assumed benefits are rarely quantified.

This work aims to comprehensively compare the performances of multi-sensor and single-sensor approaches to understand to what extent increasing the number and variegate data source may improve the detection rate and temporal characterisation of flood events. A multi-sensor flood monitoring approach using AMSR2 and VIIRS data is assessed against each sensor individually and against standard benchmarks in EO-based flood detection (e.g., MODIS and Sentinel-1)  for major flood events in the Savannakhet Province of Laos.

The comparative analysis evaluates multiple metrics. First, detection comparison classifies events as captured by each considered approach, multi-sensor only, each individual sensor only, or missed by all, to directly quantify the improvement attributable to multi-sensor integration. The spatial agreement is assessed between the multi-sensor and single sensor approaches for jointly detected flood events. Additionally, the temporal component is characterized by an examination of the observation frequency, maximum observation gaps, and peak capture timing. Lastly, the various detection outcomes are related to event characteristics, including cloud cover persistence, flood magnitude, duration, and flood type, quantifying the conditions under which a multi-sensor approach performs optimally.

How to cite: Campo, C., Tamagnone, P., Schumann, G., Duc Tran, T., Choy, S., and Kuleshov, Y.: Comprehensive validation of the benefits of multi-sensor flood monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20097, https://doi.org/10.5194/egusphere-egu26-20097, 2026.

Integrated Monitoring of Lake Garda with Radar, Optical Sensors and In Situ Instruments: Insights from the SARLAKES Project

Virginia Zamparelli1, Simona Verde1, Andrea Petrossi1, Gianfranco Fornaro1, Marina Amadori2,3, Mariano Bresciani2, Giacomo De Carolis2, Francesca De Santi4, Matteo De Vincenzi3, Giulio Dolcetti3, Ali Farrokhi3, Raffaella Frank2, Nicola Ghirardi2,5, Claudia Giardino2, Fulvio Gentilin6, Alessandro Oggioni2, Marco Papetti6, Gianluca Pari7 Andrea Pellegrino2, Sebastiano Piccolroaz3, Tazio Strozzi8, Marco Toffolon3, Maria Virelli7, Nestor Yague-Martinez9, and Giulia Valerio6

 

1Institute for Electromagnetic Sensing of the Environment (IREA), National Research Council, Naples, Italy

2Institute for Electromagnetic Sensing of the Environment (IREA), National Research Council, Milan, Italy

3Department of Civil, Environmental and Mechanical Engineering (DICAM), University of Trento, Trento, Italy

4Institute for Applied Mathematics and Information Technologies (IMATI), National Research Council, Milan, Italy

5 Institute for BioEconomy (IBE), National Research Council, Sesto Fiorentino, Italy

6Department of Civil, Environmental, Architectural Engineering and Mathematics (DICATAM), University of Brescia, Brescia, Italy

7Italian Space Agency (ASI), Rome, Italy

8GAMMA Remote Sensing, Gümligen, Switzerland

9Capella Space Corp., San Francisco, CA, USA

 

SARLAKES (SpatiAlly Resolved veLocity and wAves from SAR images in laKES) is a PRIN (Projects of National Interest) project funded in 2022 by the Italian Ministry of University and Research. The project is now in its final phase and is scheduled to end at the beginning of 2026. The project developed a novel, advanced and adaptable tool capable of accurately measuring water dynamics in medium- and large-sized lakes.

A key and innovative aspect of the project is the use of spaceborne Synthetic Aperture Radar (SAR) data, which are widely exploited for routine observation of the marine environments but remain relatively underutilized for lake monitoring. SARLAKES investigated the capability of SAR imagery to retrieve the spatial distribution of wind fields, surface currents, and wind-generated waves in lacustrine environments.

The project considers Lake Garda and Lake Geneva as case studies, with Lake Garda—the largest lake in Italy—selected as the primary test site due to the research group’s long-standing experience and the availability of extensive historical data.

This contribution presents the main results obtained over two years of project activity, with particular emphasis on outcomes from a multidisciplinary field campaign conducted on April 2025. The campaign aimed to reconstruct lake surface currents during a strong wind event in the peri-Alpine Lake Garda region.

The field instrumentation included a wave buoy, an acoustic Doppler current profiler (ADCP), Lagrangian drifters, anemometers, a ground-based radar, fixed cameras, a drone, and a conductivity–temperature–depth profiler. Satellite acquisitions from the COSMO-SkyMed Second Generation and Capella Space SAR sensors, as well as from the optical sensor PRISMA were scheduled over the study area during the campaign. Archive data from Sentinel-1, Sentinel-2, Sentinel-3, Landsat, and COSMO-SkyMed missions were also utilized.

The project demonstrates how the integration of in-situ instrumentation, spatially distributed flow measurements from remote sensing, and hydrodynamic modeling provides a comprehensive and scalable approach to next-generation monitoring of complex lake systems.

How to cite: Zamparelli, V. and the SARLAKES project team: Integrated Monitoring of Lake Garda with Radar, Optical Sensors and In Situ Instruments: Insights from the SARLAKES Project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21000, https://doi.org/10.5194/egusphere-egu26-21000, 2026.

Semi-urban vegetation systems play a critical role in ecosystem stability but are increasingly exposed to flood hazards due to climate variability and rapid land-use change. Accurate flood detection in such system remains challenging because radar backscatter is influenced by complex and mixed scattering mechanisms arising from vegetation, built-up structures, and surface water. Conventional intensity-based flood indices struggle to separate flooded vegetation from non-flooded rough surfaces and tend to miss inundated areas under mixed land-cover conditions. To address these limitations, this study presents a physically interpretable flood detection framework that integrates Synthetic Aperture Radar polarimetric descriptors with a machine learning classifier. The proposed approach utilizes dual-polarized Sentinel-1 SAR data to derive polarimetric features from Stokes parameters and the covariance matrix. Specifically, the Degree of Polarization and Linear Polarization Ratio are combined with eigenvalue-based information to capture changes in both amplitude and polarization state between pre-flood and during-flood conditions. These descriptors are integrated into a novel Flood Index (FI) designed to distinguish flooded urban areas dominated by double-bounce scattering from flooded vegetation characterized by depolarized volume scattering. Unlike commonly used indices such as the Normalized Difference Flood Index (NDFI) or VH/VV ratio, the proposed FI exploits polarization behaviour rather than relying solely on backscatter intensity. A Random Forest classifier is trained on the proposed FI using a tile-based sampling strategy to handle class imbalance between flooded and non-flooded pixels. The framework is evaluated across three flood events representing diverse geographic and land-cover conditions: the 2019 Typhoon Hagibis flood in Japan, the 2023 Yamuna River flood in India, and the 2023 Larissa flood in Greece. Model performance is assessed using multiple accuracy metrics, including F1 score, Intersection over Union (IoU), False Positive Rate (FPR), and False Negative Rate (FNR). Results demonstrate that the Random Forest model trained on the proposed Flood Index consistently outperforms threshold-based Otsu methods and NDFI across all study areas. The approach achieves F1 scores ranging from 0.81 to 0.86 and IoU values between 0.70 and 0.76, while maintaining a relatively low False Negative Rate (0.09-0.17), that is critical for minimizing missed flooded areas in disaster response applications. Sensitivity and ablation analyses further confirm the robustness of the Flood Index to speckle noise and highlight the complementary contribution of its individual components. Overall, the proposed framework offers a transferable and computationally efficient solution for flood mapping in semi-urban vegetation systems using widely available dual-polarized SAR data. The results highlight its potential for scalable flood monitoring and rapid damage assessment across regions with heterogeneous land-cover conditions.

How to cite: Adhikari, R. and Bhardwaj, A.: SAR polarimetry-based machine learning method for flood detection in semi-urban vegetation systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21063, https://doi.org/10.5194/egusphere-egu26-21063, 2026.

EGU26-21507 | ECS | Posters on site | HS6.5

Flood Susceptibility Mapping with GFI 2.0 and Artificial Intelligence Models 

Jorge Saavedra Navarro, Ruodan Zhuang, Caterina Samela, and Salvatore Manfreda

Floods are among the most damaging natural hazards, motivating the development of rapid and scalable tools for floodplain mapping across multiple return periods and for post-event assessment. The Geomorphic Flood Index (GFI) is widely used to identify flood-prone areas using topographic information, but it can exhibit reduced reliability under complex hydraulic conditions—particularly near confluences where backwater controls water levels—and it may systematically overestimate inundation extents when used as a binary classifier.

This study advances the GFI framework by explicitly accounting for backwater effects at river confluences and along tributary junctions. In parallel, to reduce the intrinsic overestimation of GFI-derived floodplains, we test a suite of Artificial Intelligence (AI) classifiers—Random Forest, XGBoost, and Neural Networks—trained through a multi-parametric formulation that combines GFI with auxiliary predictors, including precipitation, lithology, land use, and slope. The approach is evaluated across multiple Italian catchments, using satellite-derived inundation and hydrodynamic simulations as independent benchmarks. Model performance is quantified against the baseline GFI approach using a standard threshold-based binary classification using an optimal cutoff.

The proposed framework aims to improve post-event flood delineation under observational constraints (e.g., satellite data gaps due to cloud cover, vegetation, or imaging limitations) and to provide a computationally efficient surrogate for extending hydrodynamic information to additional return periods or large basins where full numerical modelling is impractical. Preliminary results indicate that Random Forest provides the most robust performance across study sites. Incorporating backwater effects yields clear gains at confluences, primarily by reducing omission errors and improving the representation of hydraulically controlled inundation patterns. Moreover, the AI-based correction substantially mitigates the overestimation typically associated with standard GFI mapping, resulting in floodplain delineations that are more consistent with complex hydrodynamic processes and suitable for scalable flood hazard applications.

How to cite: Saavedra Navarro, J., Zhuang, R., Samela, C., and Manfreda, S.: Flood Susceptibility Mapping with GFI 2.0 and Artificial Intelligence Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21507, https://doi.org/10.5194/egusphere-egu26-21507, 2026.

EGU26-21622 | ECS | Orals | HS6.5

Mapping and modeling coastal flood dynamics using remote sensing and hydrodynamic models 

Giovanni Fasciglione, Guido Benassai, Gaia Mattei, and Pietro Patrizio Ciro Aucelli

This study presents an integrated and multidisciplinary methodology for investigating coastal flooding and morphodynamic processes in low-lying coastal environments, with a comparative application to two geomorphologically distinct Mediterranean coastal plains: the Volturno Plain and the Fondi Plain. The methodological framework combines high-resolution topographic and bathymetric datasets, aerial remote sensing, sedimentological analyses, statistical wave climate assessment, numerical hydrodynamic modelling, and relative sea-level rise scenarios that incorporate both eustatic trends and local vertical land movements. This approach enables a robust evaluation of how differing coastal configurations influence flooding susceptibility under extreme marine conditions.

For both study areas, the topographic baseline was derived from 2 m resolution LiDAR-based Digital Terrain Models, subsequently refined using site-specific datasets. In the Volturno Plain, extensive GNSS field surveys were conducted along the beach between Volturno and Regi Lagni river mouths. In the Fondi Plain, DTM refinement relied on aerial drone surveys carried out over the beach sector between the Canneto and Sant’Anastasia river mouths. Photogrammetric processing of aerial imagery allowed the generation of high-resolution surface models, which were integrated with the existing LiDAR DTM to enhance the depiction of subtle morphological features critical for flood propagation.

Sedimentological characterization was performed to constrain morphodynamic responses. Granulometric samples were collected along cross-shore transects at elevations ranging from −1.5 m to +2 m. Grain-size distribution analyses supported the calibration and interpretation of sediment transport and wave dissipation processes within numerical models.

Bathymetric modelling was based on high-precision single-beam echo-sounder surveys, with depth data corrected for tidal variations using official tide-gauge records. Emerged and submerged datasets were merged into continuous topo-bathymetric models, ensuring consistency in vertical reference systems and numerical stability.

Marine storms were identified through the analysis of offshore buoy records using a Peak Over Threshold approach. Storm events were classified into five classes using their Storm Power Index calculated by combining significant wave height and event duration. Representative events were selected as boundary conditions for coupled hydrodynamic simulations performed with Delft3D and XBeach. Simulations were run for future scenarios based on high-emission IPCC projections (SSP 5-8.5), integrating local sea-level rise, local subsidence rates, and highest tidal and surge levels.

A comparative analysis of the simulation outcomes highlights marked differences between the two coastal plains. The Volturno Plain results highly prone to inundation, with storm surges overtopping dune systems and propagating inland due to low elevations, local subsidence, and limited effectiveness of existing coastal defenses. Conversely, the Fondi Plain exhibits significantly reduced flood penetration. The presence of a wide bar system, coupled with efficient coastal defense structures, promotes substantial dissipation of incoming wave energy. As a result, even under intense storm conditions, inundation remains confined to a narrow coastal strip immediately landward of the beach.

Overall, the comparative methodological application demonstrates how coastal morphology, sedimentological properties, and defense systems critically control flood dynamics. The proposed framework provides a transferable and decision-oriented tool for assessing coastal vulnerability and supporting adaptation strategies in heterogeneous low-lying coastal settings under climate change pressure.

How to cite: Fasciglione, G., Benassai, G., Mattei, G., and Aucelli, P. P. C.: Mapping and modeling coastal flood dynamics using remote sensing and hydrodynamic models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21622, https://doi.org/10.5194/egusphere-egu26-21622, 2026.

EGU26-21631 | ECS | Posters on site | HS6.5

Assessment of Multi-Mission Satellite Altimetry GDR L2 Products for River Water Surface Elevation in the Ganga Basin 

Barun Kumar, Shyam Bihari Dwivedi, and Shishir Gaur

Precise monitoring of water surface elevation (WSE) in data-deficient areas such as the Ganga River stretch is essential for hydrological modelling, flood prediction, and comprehensive water resource management. This study introduces a comprehensive evaluation framework for Level-2 Geophysical Data Records (GDR L2) derived from various satellite altimetry missions, including Sentinel-3A/B, Sentinel-6A, Jason-3, and SWOT Nadir, validated against in-situ gauge stations from the Central Water Commission (CWC) across a range of hydrological conditions. The process includes advanced geographical analysis. Gaussian-process Kriging interpolation generates continuous longitudinal WSE profiles across strategically placed virtual stations; rigorous outlier detection employs interquartile range (IQR) and Hampel filters; bias correction employs dry-season median alignment to a common orthometric datum; and Kalman filter smoothing effectively reduces measurement noise while preserving critical hydrological signal dynamics.

Comprehensive performance evaluations employ co-located time series analysis, scatter plots, and flow duration curves (FDCs), with seasonal stratification distinguishing monsoon high-flow variability from stable non-monsoon baseflow conditions. The evaluation stresses physically significant parameters based on Kling-Gupta Efficiency (KGE) and RMSE. Sentinel-6A is the strongest performer in all situations with high non-monsoon accuracy (KGE 0.894, RMSE 0.089 m) and monsoon performance (KGE 0.57, RMSE 3.08 m) despite turbulent flow issues, but SWOT Nadir's processing potential is limited by specific hooking artifacts. During non-monsoon periods, measurement reliability is consistently 2-4 times higher. This proven multi-mission system demonstrates satellite altimetry as an operationally viable method for WSE retrieval in major braided rivers, allowing for accurate rating curve generation and discharge computation. In future machine learning data fusion and hydrodynamic modelling can be incorporated to increase basin-scale forecast capabilities.

How to cite: Kumar, B., Dwivedi, S. B., and Gaur, S.: Assessment of Multi-Mission Satellite Altimetry GDR L2 Products for River Water Surface Elevation in the Ganga Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21631, https://doi.org/10.5194/egusphere-egu26-21631, 2026.

EGU26-21734 | Posters on site | HS6.5

Evaluating Copernicus Global Flood Monitoring (GFM) Service trade-offs in near-real-time flood mapping 

Shagun Garg, Ningxin He, Sivasakthy Selvakumaran, and Edoardo Borgomeo

Near-real-time satellite-based flood maps support disaster risk management and emergency response. One widely used service is the Global Flood Monitoring (GFM) product of the Copernicus Emergency Management Service, launched in 2021 and based on Sentinel-1 Synthetic Aperture Radar (SAR) data. The GFM service combines three flood-mapping algorithms: pixel-based thresholding, region-based approaches, and change-detection techniques, merged using a majority-voting scheme to generate the final flood extent product. Another key strength of the GFM service is its rapid analysis, providing flood maps within approximately five hours of satellite image acquisition through a fully automated processing chain. As the product is increasingly relied upon by practitioners and decision-makers, there is a growing need to assess its accuracy and robustness. Understanding false alarms and missed detections is critical for improving the reliability and usability of the service.


In this study, we systematically compare GFM flood maps across twenty real-world flood events using high-resolution reference datasets. To ensure temporal consistency, the GFM-derived flood maps are generated using Sentinel-1 acquisitions from the same day as the reference observations. Spatial agreement between datasets is quantified using the Intersection-over-Union metric.


Our results suggest that the GFM service performs well for large, extensive flood events but degrades for smaller, localized ones. Many of the observed errors come not from flood detection itself, but from inaccuracies in the reference water layer - while surface water is correctly identified, misclassification of permanent or seasonal water bodies leads to false alarms and missed floods. We evaluate the three-underlying flood-mapping algorithms individually for consistent patterns of misdetection or false alarms. In addition, we develop an automated framework to rapidly compare any external flood map with the GFM outputs, enabling near-instant evaluation of agreement and error patterns. 


This framework provides practical insights into where and why the GFM services achieve successes and failures and offers continuous validation and iterative improvement of global flood mapping services. 

How to cite: Garg, S., He, N., Selvakumaran, S., and Borgomeo, E.: Evaluating Copernicus Global Flood Monitoring (GFM) Service trade-offs in near-real-time flood mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21734, https://doi.org/10.5194/egusphere-egu26-21734, 2026.

EGU26-22077 | Orals | HS6.5

A fully automatic processing chain for the systematic monitoring of surface water using Copernicus Sentinel 1 satellite data: first results of the SCO-CASCADES project. 

Renaud Hostache, Cyprien Alexandre, Chhenglang Heng, Thibault Catry, Vincent Herbreteau, Vannak Ann, Christophe Révillion, and Carole Delenne

Water is essential to life and health of various ecological and social systems. Unfortunately, water is one of the natural resources most impacted by climate change, with increasingly intense hydro-meteorological extremes (floods, droughts, etc.) and growing societal demand. To help manage this vulnerable resource, it is vital to assess and monitor its availability on a regular basis, as well as to track its trajectory over time to better understand the impact of global change on it. Surface water (lakes, rivers, flood plains, etc.) represents an important component of total water resources, and it is of primary importance to monitor it to better understand and manage the consequences of climate change. Surface water resources provide populations around the world with essential ecosystem services such as power generation, irrigation, drinking water for humans and livestock, and space for farming and fishing.

In this context, the SCO-CASCADES project implements end-to-end processing chains for satellite Earth observation data, including Sentinel-1 and 2 (S-1 and S-2), in order to provide surface water products (surface water body and inundation depth maps) that will be made available via an interactive platform co-constructed with identified users.

In the first phase of the project a fully automated Sentinel-1 based processing chain has been implemented. This chain is based on automatic multiscale image histogram parameterization followed by thresholding, region growing and chain detection applied on individual, subsequent pairs, and time series of S1 images. This chain enables us to derive various products: i) an exclusion layer identifying areas where water cannot be detected on Sentinel 1 image (e.g. Urban and forested areas), ii) permanent seasonal water body maps, iii) a water body map for each S1 image, iv) an uncertainty map characterizing the water body classification uncertainty, v) an occurrence map providing the number of times (over the time series) each pixel was covered by open water.

Here, we propose to present and evaluate the robustness of the processing chain and the resulting maps produced using multi-year S1 time series over two large scale sites: the Mekong flood plains between Kratie, the Tonle Sap lake and the Mekong Delta, and the Tsiribihina basin in Madagascar. The kappa score obtained from the comparison between S1 and S2-derived maps shows a good agreement yielding CSI and Kappa Cohen scores most of the time higher than 0.7 and sometimes reaching values higher than 0.9.

How to cite: Hostache, R., Alexandre, C., Heng, C., Catry, T., Herbreteau, V., Ann, V., Révillion, C., and Delenne, C.: A fully automatic processing chain for the systematic monitoring of surface water using Copernicus Sentinel 1 satellite data: first results of the SCO-CASCADES project., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22077, https://doi.org/10.5194/egusphere-egu26-22077, 2026.

EGU26-247 | Posters on site | HS3.4

Addition of Process-Based Stream Temperature Modeling Capabilities to MODFLOW 6 

Eric Morway, Katie Fogg, Alden Provost, Christian Langevin, Joseph Hughes, and Martijn Russcher

MODFLOW is a well-known and widely used groundwater flow simulator.  Characteristics that have historically defined MODFLOW remain in place: it is open-source, freely available, well-documented, and intuitive.  A complete rewrite of MODFLOW in 2017 has facilitated the adoption of several new model types embedded directly into the MODFLOW framework.  In addition to simulating groundwater flow, MODFLOW 6 now also includes solute transport, particle tracking, and a new heat-transport model called the Groundwater Energy (GWE) transport model.  Many other enhancements are actively being developed.  As with all model types available within the MODFLOW 6 hydrologic simulator, the GWE model leverages the design concept commonly referred to as packages – modules that represent specific features of the hydrologic system being modeled.  For example, the Streamflow Routing (SFR) package can be activated to simulate flow in streams.  If desired, users also can simulate heat transport within a stream network by activating the Streamflow Energy (SFE) transport package.  The SFE package simulates advective heat transport within the stream network while also accounting for advective and conductive heat exchange with the underlying groundwater system.  Although the initial release of GWE offered basic heat transport functionality in stream networks through the SFE package, detailed representation of heat exchange between stream reaches and the atmosphere was not included.  However, recent SFE development efforts are focused on adding functionality to represent heat exchange with the atmosphere.  New processes by which heat may be exchanged with the atmosphere are short- and long-wave radiation and sensible and latent heat fluxes.  When finished, the new process-based stream temperature modeling capabilities will work with the other MODFLOW features, including the application programming interface (API), parallel simulation, the input data model (IDM), and support within the popular FloPy Python library.

How to cite: Morway, E., Fogg, K., Provost, A., Langevin, C., Hughes, J., and Russcher, M.: Addition of Process-Based Stream Temperature Modeling Capabilities to MODFLOW 6, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-247, https://doi.org/10.5194/egusphere-egu26-247, 2026.

EGU26-1167 | ECS | Posters on site | HS3.4

Enhancing Streamflow Simulations Through Input Data Denoising 

Injila Hamid and Vinayakam Jothiprakash

Hydrological models are vital for understanding water resources and their responses to environmental and climatic changes, but their accuracy depends strongly on input data quality. This study evaluates how noise reduction in meteorological inputs influences the performance of the SWAT hydrological model for the lower Columbia River basin. Wavelet Transform (WT) was applied for partial denoising, while Singular Spectrum Analysis (SSA) was used for both partial and full noise removal. SSA allows extraction of trend, periodic, and noise components individually from time series data. Results indicate that partial denoising using WT significantly improves model performance, increasing the correlation coefficient (r) and Nash–Sutcliffe Efficiency (NSE) by 2 to 5%, Kling-Gupta Efficiency (KGE) by 16%, and reducing RSR by 4%, along with a notable reduction in PBIAS (from −4.7 to +1.3). The partially denoised WT model achieved r = 0.91, NSE = 0.81, PBIAS = 1.30, KGE = 0.88, and RSR = 0.45, outperforming both the base and fully denoised models. The comparative analysis shows that completely removing noise offers limited benefits and may suppress natural variability, while partial denoising provides an optimal balance between data reliability and model precision. These findings highlight the importance of appropriate input-data preprocessing in improving hydrological model performance and reducing uncertainty in water resource assessments.

How to cite: Hamid, I. and Jothiprakash, V.: Enhancing Streamflow Simulations Through Input Data Denoising, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1167, https://doi.org/10.5194/egusphere-egu26-1167, 2026.

EGU26-1351 | ECS | Orals | HS3.4

Geostatistical active learning for expanding monitoring networks for environmental decision making 

Felix Henkel, Jonathan Frank, Thomas Suesse, and Alexander Brenning

The expansion and optimisation of environmental monitoring networks requires the efficient use of limited resources to improve spatial predictions to ensure the protection of human health and ecosystems.

Network densification is a spatial sampling problem that is often addressed by pointwise-prediction uncertainty approaches, which ignore (1) the impact of a new site on its neighbourhood and (2) the binary decision task motivating the monitoring. Active learning (AL) is a machine learning technique that iteratively selects new locations based on the current maximum uncertainty in the available training data. We therefore recast network densification as an AL task and propose model-agnostic acquisition criteria, including a decision-aligned focal logit criterion that prioritises neighbourhoods whose exceedance probabilities lie near regulatory thresholds. A look-ahead criterion based on the expected reduction in prediction standard error (SE) is also examined. In a groundwater nitrate concentration case study, the focal logit criterion consistently selected more informative sites than traditional dispersion- or prediction-SE-based criteria, yielding up to 58 % greater gains in exceedance-mapping accuracy (Cohen’s κ)). Focal logit and SE criteria outperformed pointwise counterparts by ~45 % on average, while the look-ahead criterion performed well but at much higher computational cost.

The proposed framework is simple, generalisable to other environmental pollutants (such as air pollutants), and supports a transparent, decision-oriented monitoring design.

How to cite: Henkel, F., Frank, J., Suesse, T., and Brenning, A.: Geostatistical active learning for expanding monitoring networks for environmental decision making, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1351, https://doi.org/10.5194/egusphere-egu26-1351, 2026.

Decisions concerning the management of natural resources are often based on binary criteria that determine whether a specific environmental target is met or exceeded. A common example is the designation of “polluted” areas, where mitigation measures must be implemented once concentrations surpass a regulatory threshold. In practice, maps of such exceedances are commonly derived from regionalized concentration estimates. However, most conventional spatial interpolation and prediction procedures introduce systematic bias in the estimated extent of polluted areas.

To overcome this issue, we apply a bias-corrected mapping procedure that is compatible with any geostatistical or machine learning method capable of providing valid probability estimates. For the case study, we mainly focus on a trans-Gaussian regression-kriging (TRGK) framework, selected for its interpretability and transparent decomposition of predictions. To assess the potential added value of nonparametric approaches, we additionally compare TRGK with quantile regression forest (QRF) in a sub-region.

The TRGK model follows a structured, non-stationary design: (i) raw concentrations are transformed to log10 scale; (ii) a nationwide global linear model captures broad-scale relationships; (iii) major hydrogeological districts serve as units for local linear refinements to account for non-stationarity; (iv) residuals are transformed using a Gaussian anamorphosis; and (v) the transformed residuals are interpolated via ordinary kriging, from which probability estimates are derived. This setup improves flexibility while maintaining interpretability and coherent uncertainty quantification.

Bias correction is performed by estimating the total exceedance area implied by the data and determining a calibrated probability threshold that ensures an unbiased delineation of the polluted area. In this study, we jointly evaluate a threshold exceedance criterion and a temporal trend criterion.

Groundwater nitrate mapping at national scale represents a challenging test case due to strong non-normality, spatial heterogeneity, and pronounced non-stationarity. The approach nonetheless performs robustly. Linear model components exhibit R2 values between 0.15 and 0.62, while semivariogram practical ranges vary from 0.3 to 22.3 km. In the sub-region comparison, QRF showed a small discrimination advantage over TRGK (AUC 0.86 vs. 0.82) but relied more heavily on calibration (underestimation without calibration 94.9% vs. 5.1%).

Overall, the results demonstrate that the bias-corrected probability-based framework provides a flexible, robust and- when coupled with geostatistics- transparent solution for large-scale pollution mapping.

How to cite: Frank, J., Suesse, T., Jiang, S., and Brenning, A.: Bias-corrected pollution mapping with non-stationary geostatistics and spatial machine learning for environmental decision making: The case of groundwater nitrate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1406, https://doi.org/10.5194/egusphere-egu26-1406, 2026.

Hydrological extreme records in many regions in the world may include observations from different genesis and levels of extremeness forming a characteristic “separation phenomenon’ that limits the effectiveness of traditional distributions such as the Gumbel and log-Pearson Type III models, and in such mixed extreme populations, the Two-Component Extreme Value (TCEV) distribution is better suited. However, conventional fitting approaches tend to emphasize the abundant ordinary data because of the scarcity of right-tail observations, which results in inaccurate predictions of high quantiles. Nevertheless, accurate representation of the upper tail (i.e., the high-value ranges of the cumulative distribution function, CDF) is essential for flood risk evaluation and the design of hydraulic structures. To address this issue, this study introduces a new TCEV fitting approach (SR-MWS) aimed at improving right-tail performance. In the new proposal, the dataset is first approximated using a piecewise two linear regression, and the slope ratio between the two parts (R = S1/S2) is used to assess whether TCEV modeling is appropriate or not (if R > 1.5, the dataset is regarded as suitable for TCEV fitting). Following, three weighting strategies—linear, quadratic, and exponential—are applied sequentially to obtain the final TCEV parameters. A partitioned scoring framework is then used to select the most suitable weighting scheme, emphasizing the mid-to-upper CDF range F(x) ∈ [0.6, 1.0], which corresponds to return periods from about 2.5 years to more than 200 years, while also considering overall fit quality. Our results show that the proposed method yields more accurate estimates for extreme values than conventional techniques and exhibits consistent performance for both peak-flow and precipitation datasets. Beyond hydrological applications, it provides an automated and robust tool for modeling extreme events and supporting risk assessment in fields characterized by mixed-population data with a pronounced dog-leg structure.

How to cite: Valdes-Abellan, J., Ta, L., and Yu, C.: New Proposal for maximum hydrological events fitting showing the ‘separation phenomenon’ with flexible TCEV Distribution , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1449, https://doi.org/10.5194/egusphere-egu26-1449, 2026.

EGU26-1813 | Orals | HS3.4

Residual error modelling for hourly streamflow predictions 

Cristina Prieto, Dmitri Kavetski, Fabrizio Fenicia, James Kirchner, David McInerney, Mark Thyer, and César Álvarez

 Statistical residual error modelling for hourly streamflow predictions

Cristina Prieto1,2,3, Dmitri Kavetski4,1, Fabrizio Fenicia3, James Kirchner2,5,6, David McInerney4, Mark Thyer4, and César Álvarez1

 

(1) IHCantabria—Instituto de Hidráulica Ambiental de la Universidad de Cantabria, Santander, Spain

(2) Department of Environmental Systems Science, ETH Zürich, Zürich, Switzerland

(3) Eawag, Swiss Federal Institute of Aquatic Science and Technology, Dübendorf, Switzerland

(4) School of Civil, Environmental and Mining Engineering, University of Adelaide, Adelaide, SA, Australia

(5) Swiss Federal Research Institute WSL, Birmensdorf, Switzerland

(6) Department of Earth and Planetary Science, University of California, Berkeley, California, USA

 

Water plays a critical role in societal stability through both its excess and scarcity. Extreme hydrological events can cause substantial human and economic losses, while water scarcity affects essential services such as drinking water supply, food production, and hydropower generation. Reliable streamflow predictions are therefore fundamental for environmental assessments, flood risk management, and Integrated Water Resources Management (IWRM).

Hydrological models are central tools for understanding catchment behaviour and generating predictions to support water-resources assessment, planning, and management. However, their predictive performance strongly depends on the temporal resolution at which they are applied.

At hourly time scales, hydrological processes and associated uncertainties become markedly more complex, particularly in small and mesoscale catchments. Flood peaks may last only a few hours, so daily streamflow predictions can substantially underestimate peak magnitudes; antecedent wetness conditions can evolve rapidly; and the dominant processes controlling short-term streamflow dynamics differ from those governing longer term behavior. For example, over longer time scales, predictions are primarily constrained by mass balance, whereas short-term predictions depend more strongly on dynamics and flow routing.

In addition to classical sources of uncertainty related to data, model structure, and parameters, hourly streamflow predictions often exhibit bias, heteroscedasticity, temporal autocorrelation, and non-stationarity.

Despite their importance, hourly streamflow prediction and uncertainty characterisation have received comparatively less attention than daily-scale studies.

In this work, we use a conceptual hydrological model to generate deterministic hourly streamflow predictions and quantify predictive uncertainty using a residual error modelling framework. Case-study catchments include hydrologically diverse basins in Europe and the United States. Bias, heteroscedasticity, and temporal dependence in model residuals are addressed using Box–Cox transformations and autoregressive and moving average (ARMA) models.

Results indicate that a logarithmic transformation combined with an autoregressive model of order three (AR(3)) provides the most consistent performance across catchments. This work advances streamflow prediction by developing statistically rigorous methods for post-processing the residuals of conceptual hydrological models at the hourly time scale, supporting more reliable hourly streamflow predictions for integrated water resources management and decision-making.

How to cite: Prieto, C., Kavetski, D., Fenicia, F., Kirchner, J., McInerney, D., Thyer, M., and Álvarez, C.: Residual error modelling for hourly streamflow predictions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1813, https://doi.org/10.5194/egusphere-egu26-1813, 2026.

EGU26-3193 | ECS | Orals | HS3.4

Designing Sampling Strategies for the Efficient Estimation of Parameterized Spatial Covariance Models 

Olivia L. Walbert, Frederik J. Simons, Arthur P. Guillaumin, and Sofia C. Olhede

Spatial data in the Earth and environmental sciences acquired by instrument collection or simulation are constrained to finite, discrete, (ir)regular grids whose geometry is delineated by a boundary within which missingness, either random or structured, may exist. We model (ir)regularly sampled Cartesian spatial data as realizations of discrete two- and three-dimensional random fields whose covariance structure we estimate parametrically with a spectral-domain maximum-likelihood estimation strategy using the debiased Whittle likelihood, which efficiently counters the effects of aliasing and spectral leakage that arise from finite sampling and boundary effects. We work with the general, flexible Matérn class of covariance functions, which characterizes the shape of a field through three parameters that quantify its amplitude, smoothness, and correlation length. We quantify parameter covariance analytically and asymptotically based on the parametric model and sampling grid alone, agnostic of observed data. Our uncertainty quantification allows us to study how sampling geometry imparts uncertainty on a covariance model and provides a path for optimizing the design of a sampling grid to reduce error for an anticipated model. We formulate several approaches for interrogating our model residuals to interpret where real Earth data depart from the null hypotheses of Gaussianity, stationarity, and isotropy. We explore select case studies that demonstrate the broad applicability of our models across Earth science disciplines and develop software in MATLAB and Python for implementation by domain scientists, in hydrology, and elsewhere.

How to cite: Walbert, O. L., Simons, F. J., Guillaumin, A. P., and Olhede, S. C.: Designing Sampling Strategies for the Efficient Estimation of Parameterized Spatial Covariance Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3193, https://doi.org/10.5194/egusphere-egu26-3193, 2026.

Spatial and temporal datasets that comprise distributions of events along a transect/timeline together with their magnitudes can display scale-dependent changes in persistence or anti-persistence that may contain signatures of underlying physical processes. Lacunarity is a technique that was originally developed for multiscale analysis of data and characterizes the distribution of spaces or gaps in a pattern as a function of scale. In this study, we demonstrate how lacunarity may be modified in order to reveal scale-dependent changes in 1-dimensional data related to fractures, sedimentary layering and rainfall. In order to address whether fractures found along a 1-dimensional transect (scanline) occur in clusters, we compare the lacunarity of a given fracture-spacing data to a theoretical random lacunarity curve. Further, we introduce the concept of 1st derivative of log-transformed lacunarity and demonstrate that this function can find the inter-cluster spacing and possible fractal behaviour over certain scales. It will be demonstrated how this same technique may be applied to a time-series, e.g., rainfall data, to see whether such events occur in clusters over certain time-scales. Next, the “event magnitudes” (e.g., fracture aperture) were added to each event data point (e.g., fracture) thus, yielding a 1-dimensional non-binary dataset and it was tested whether the dataset shows scale-dependent changes in terms of anti-persistence and persistence. The concept of lacunarity ratio, LR, is introduced, which is the lacunarity of a given dataset normalized to the lacunarity of its random counterpart. This randomization however, is different from the one used in the previous technique. In case of our fracture dataset for example, the random sequence is generated by leaving the locations of fractures unaltered and randomly reallocating the magnitudes along the dataset. It was demonstrated that LR can successfully delineate scale-dependent changes in terms of anti-persistence and persistence. In addition to the fracture data already mentioned here (spacing and apertures from NE Mexico), the one used for developing this technique, it was applied to two different types of data: a set of varved sediments from Marca Shale and, a hundred-year rainfall record from Knoxville, TN, USA. While the fracture data showed anti-persistence at small scales (within cluster) and random behavior at large scales, the rainfall data and varved sediments both appear to be persistent at small scales becoming random at larger scales. It was no surprise to find such striking similarity between the spatial “sedimentary” data and the time-dependent rainfall data because in rock records, the former is often considered to be a proxy for the latter. In general, such differences in behavior with respect to scale-dependent changes in anti-persistence to random, persistence to random, or otherwise, maybe be related to differences in the physicochemical properties and processes contributing to multiscale datasets.

How to cite: Roy, A. and Mukerji, T.: Identifying Scale-dependent Spatial and Temporal Patterns in Earth Science Data: Lacunarity-based Techniques, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4505, https://doi.org/10.5194/egusphere-egu26-4505, 2026.

EGU26-5236 | Orals | HS3.4

Which grid points are statistically significant? Revisiting false discovery rate correction in geospatial data 

Michael Schutte, Leonardo Olivetti, and Gabriele Messori

Scientific publications in the geosciences routinely assess statistical significance in spatially distributed environmental and geophysical data. When statistical significance is indicated, it is most often assessed independently at each grid point, while formal adjustment for multiple testing is rarely applied. However, applying multiple testing corrections, such as the global false discovery rate (FDR) approach is not always straightforward, as environmental and geophysical data are often spatially correlated.

In our work, we highlight how neglecting multiple testing correction can substantially inflate the number of false positives. We further show that commonly used FDR implementations can yield counterintuitive and potentially misleading results when applied to strongly spatially correlated data.

To illustrate the latter point, we provide an example based on near-surface air temperature composites following sudden stratospheric warmings. We first show that when anomalies are spatially coherent, restricting the spatial domain can increase the FDR-adjusted significance threshold. As a result, the same underlying field may display a larger share of statistically significant grid points solely due to domain selection. We analyze the origin of this behavior from a rank-based perspective and discuss its implications for spatial inference and uncertainty quantification in environmental sciences.

Based on these insights, we propose practical recommendations for robust and transparent significance assessment, such as spatially aggregated or spatially aware alternatives. Our results highlight both the need to account for multiple-testing and potential issues with a naïve application and interpretation of FDR correction. While illustrated using atmospheric data, the findings are directly relevant to hydrology and other environmental sciences where statistical significance is assessed across spatial fields.

How to cite: Schutte, M., Olivetti, L., and Messori, G.: Which grid points are statistically significant? Revisiting false discovery rate correction in geospatial data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5236, https://doi.org/10.5194/egusphere-egu26-5236, 2026.

EGU26-7544 | ECS | Posters on site | HS3.4

Toward Stable Groundwater–Surface Water Coupling in Landscape Evolution Models 

Farshid Alizadeh, Raphael Bunel, Nicolas Lecoq, and Yoann Copard

Integrated landscape-evolution models require groundwater models that are computationally efficient, groundwater component that remains stable over multidecadal simulations, and strong coupling with surface hydraulics and sediment transport. In CLiDE, which is built on CAESAR–Lisflood, the backward-Euler groundwater update is simple, but as grid resolution or hydraulic diffusivity increases, it becomes highly restrictive due to the diffusion-type Courant–Friedrichs–Lewy (CFL) stability constraint. We present a redesign of CLiDE’s groundwater module that provides two complementary pathways: a behavior-preserving optimized explicit solver and a fully implicit formulation based on backward-Euler time integration. The implicit approach uses a Picard iteration to address the nonlinearity of unconfined transmissivity and the sparse symmetric positive-definite systems with a preconditioned conjugate-gradient solver. We benchmark both solvers across 25 years in fully coupled hydro-geomorphic experiments at the 104 km² Orgeval catchment in north-central France using hourly and daily groundwater coupling intervals. The implicit solver achieves a water mass balance at the catchment scale within 0.1% while remaining unconditionally stable at daily time steps and achieving solutions comparable to the hourly implicit solution. Groundwater head diagnostics are typically within 0.01 m of each other. The consistency in outlet hydrographs, inundation patterns, and long-term sediment-export behavior indicates that daily implicit coupling, in this case, can be selected based on process time scales, and not on numerical stability. Moreover, the optimized explicit solver accelerates the legacy scheme by 1.3 to 1.6 times refinements to specific algorithms, with no change in numerical outputs. Collectively, these advances enhance CLiDE's capability for additional fully coupled, long-duration simulations and suggest a preference between efficiency-oriented explicit updates and robustness-oriented implicit integration.

How to cite: Alizadeh, F., Bunel, R., Lecoq, N., and Copard, Y.: Toward Stable Groundwater–Surface Water Coupling in Landscape Evolution Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7544, https://doi.org/10.5194/egusphere-egu26-7544, 2026.

EGU26-7835 | ECS | Orals | HS3.4

Reliable Predictive Resolution in GeospatialModelling 

Meng Lu and Jiong Wang

High-resolution geospatial prediction and satellite image downscaling are increasingly enabled by advances in machine learning and the availability of fine-scale covariates. However, predicted maps are often delivered on arbitrary grids that are not justified by the sampling density of observations. While uncertainty can be quantified at unobserved locations, the spatial scales over which predictions are supported by the data and the modelling process are typically not characterized. Besides computational and storage costs, critical consequences including over-interpretation, modelling noise, and most importantly, the apparent predictive resolution of spatial products can be misleading for downstream applications, potentially affecting scientific conclusions. An example is the use of predicted air pollution maps in health cohort studies to assess exposure–response relationships. This raises a fundamental but under-addressed question: what is the finest spatial resolution at which predictions are meaningfully supported by the data (and model)?

We investigate how to meaningfully determine the predictive resolution in regression models by linking sampling density and model parameters in the frequency domain through spectral analysis. Two challenges are 1) to identify the sampling density in the multi-dimensional feature space, where the sampling typically becomes irregular; and 2) how to relate the frequency in the feature space to the spatial resolution. Using simulated and real-world geospatial datasets, we show that some arbitrarily selected output resolutions in existing literatures could exceed the data-supported predictive resolution, and could induce unnoticed biases or change-of-support issues in downstream analyses.

How to cite: Lu, M. and Wang, J.: Reliable Predictive Resolution in GeospatialModelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7835, https://doi.org/10.5194/egusphere-egu26-7835, 2026.

Stochastic rainfall models are probabilistic tools able to simulate synthetic rainfall datasets with statistical properties that resemble those from observations, which makes them particularly suitable to assess the uncertainty of rainfall estimates and to conduct sensitivity analysis of hydro-meteorological modeling chains. When the focus of the modeling is on spatial and temporal patterns, models based on space-time Gaussian random fields (GRFs) are often used because they enable modeling rainfall at any point of the space-time domain from sparse and heterogeneous data (typically observations from a rain gauge network).

In this presentation I will explore how a new model of space-time, multivariate and non-stationary GRF can be leveraged to improve stochastic rainfall modeling. A parametric transform function is combined with the GRF to account for rainfall intermittency and skewed marginal distribution, which results in a so-called trans-Gaussian (or meta-Gaussian) model. Among the many applications achieved by this flexible trans-Gaussian model I will examine how spatial non-stationarity can model orographic effects, and how multivariate modeling can be used to embed rainfall into a stochastic weather generator including five different variables (rainfall, temperature, wind, solar radiation and humidity).

How to cite: Benoit, L.: Stochastic rainfall modeling using spatio-temporal, multivariate and nonstationary trans-Gaussian random fields, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7961, https://doi.org/10.5194/egusphere-egu26-7961, 2026.

EGU26-9994 | ECS | Posters on site | HS3.4

Probabilistic mapping of groundwater nitrate pollution using a Bayesian Gaussian process model 

Kassandra Jensch, Márk Somogyvári, and Tobias Krüger

Nitrate groundwater pollution threatens the quality of drinking water and is directly linked to intensive fertiliser inputs on agricultural fields. To reduce pollution from agricultural sources, areas with, or at risk of, elevated nitrate concentrations must be designated as Nitrate Vulnerable Zones (NVZs) under the European Nitrates Directive. In Germany, as elsewhere in Europe, the designation of NVZs follows a binary classification scheme that does not account for uncertainties in the underlying data and interpolation method. We present an alternative geostatistical framework that explicitly introduces uncertainties into the established designation framework, enabling a more accurate assessment of nitrate groundwater pollution. Using a Bayesian Gaussian process model, nitrate concentrations in groundwater were predicted across the federal state of Brandenburg, Germany, where nitrate pollution is an acute problem. Our model specifically incorporates measurement errors as well as systematic biases from different observation types. The model allows for the calculation of exceedance probabilities which provides a continuous representation of nitrate pollution risk across space, relative to the legal nitrate limit of 50 mg/L. We show that the majority of agricultural land in the study area has at least a 50% probability of exceeding this limit. Additionally, measurement errors were identified as the main source of uncertainty in estimated nitrate concentrations, leading to relatively wide posterior predictive distributions. The results indicate that areas with high exceedance probability extend beyond currently designated NVZs. Unlike the established designation workflow, the proposed approach accounts for the complex reality and uncertainty of nitrate pollution in groundwater and can be readily extended to other countries in the EU and beyond. This enables a more robust and transparent designation of NVZs, and demonstrates the value of explicitly incorporating uncertainty into environmental modelling in high-profile policy settings.

How to cite: Jensch, K., Somogyvári, M., and Krüger, T.: Probabilistic mapping of groundwater nitrate pollution using a Bayesian Gaussian process model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9994, https://doi.org/10.5194/egusphere-egu26-9994, 2026.

EGU26-12514 | ECS | Orals | HS3.4

How environmental conditions influence satellite detection of rainfall events 

Chun Zhou, Li Zhou, Luca Brocca, and Dui Huang

Precipitation serves as a critical link between climate and hydrology, with variability shaped by environmental factors that regulate satellite detection under complex conditions. Physical response mechanisms under varying temperature, soil moisture, and pressure remain insufficiently assessed. Using global gauge precipitation and ERA5-Land reanalysis data, we identified HIT, MISS, FALSE events and examined their differential responses to key environmental variables. We demonstrate that HIT events tend to occur under intermediate environmental conditions, with both products sharing similar responses but GSMaP exhibiting slightly smoother temperature signals and IMERG stronger soil-moisture-related variability. MISS events, linked to colder, wetter backgrounds, are associated with larger spread, while FALSE events arise mainly in warm, dry regimes with low soil moisture and more fluctuations in IMERG. Environmental factors modulate detection, with warmer and wetter conditions favoring HIT and suppressing FALSE, while pressure plays a weaker, secondary role. These findings support satellite-based global hydrology and climate-resilience assessment.

How to cite: Zhou, C., Zhou, L., Brocca, L., and Huang, D.: How environmental conditions influence satellite detection of rainfall events, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12514, https://doi.org/10.5194/egusphere-egu26-12514, 2026.

EGU26-13518 | Orals | HS3.4

Trend or persistence: what are we really detecting in annual low-flow time series? 

Gregor Laaha and Johannes Laimighofer

Trends in annual low-flow time series are central to water resources and drought management, yet estimates are strongly affected by serial persistence, and dependence can make persistence appear as trend. We compare nonparametric and parametric methods under short-term autocorrelation and long-term persistence (LTP) and evaluate their reliability with European streamflow data and simulation-based experiments.

For short-term autocorrelation, modified Mann–Kendall approaches with block-bootstrap-based significance correction (BBSMK) and simultaneous bias-corrected prewhitening yield robust results; alternative variants inflate significance and produce implausible findings. Parametric ARIMAX models indicate that, when analyses are based on the water year, only a small share of series require higher autoregressive orders, whereas calendar-year aggregation induces more complex correlation structures and, in turn, unreliable (too low) significance rates.

Under long-term dependence, the nonparametric Mann–Kendall–LTP approach markedly lowers the fraction of significant trends, while FARIMAX models (external trend + LTP) produce similar rates to BBSMK. Yet AIC-based selection typically replaces LTP with short-term autocorrelation, indicating that what appears as persistence is often explainable by short-range dependence.

We finally assess misclassification in parametric and nonparametric trend models under LTP using nature-based simulations across record lengths. Calibrated to stream-gauge records, the simulations test whether series with deterministic trends and short-term autocorrelation—but without true LTP—are misclassified as LTP, and how such misclassification biases trend estimates. Across four scenarios (high/low LTP × significant/non-significant trend), LTP misclassification and trend-detection errors are elevated: with a trend present, short-term autocorrelation is often mistaken for LTP, biasing estimates and reducing power. At hydrologically typical record lengths, errors remain substantial, declining only for extremely long series (1,000–10,000 years); misclassification of short-term correlation as LTP persists even then.

Overall, under common record lengths and dependence structures, deterministic trends are often misinterpreted as long-term persistence—and, conversely, genuine persistence can be mistaken for trend. Therefore, LTP-based trend analyses should be interpreted with caution; typical hydrological records are too short for reliable LTP inference.

How to cite: Laaha, G. and Laimighofer, J.: Trend or persistence: what are we really detecting in annual low-flow time series?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13518, https://doi.org/10.5194/egusphere-egu26-13518, 2026.

This study investigates multilevel flood susceptibility mapping at the national scale in North Macedonia, utilizing 328 historical flood events, 14 conditioning factors derived from a digital elevation model, simplified lithology, and computed direct runoff. The methodology integrates fuzzy set theory (Fuzzy), analytic hierarchy process (AHP), weighted linear combination (WLC), and random forest (RF) approaches. The two-stage process employs distinct sets of conditioning factors in sequential flood susceptibility mapping: first, generating Fuzzy/AHP/WLC predictions and pseudo-absence data, and second, producing five RF predictions by varying pseudo-absences and binary cutoffs. Validation results indicate that the very high susceptibility class (0.8–1.0) of the Fuzzy/AHP/WLC model predicted 46.6% of flood pixels within 31.6% of the total area. In comparison, the very high susceptibility class of the RF models predicted 88.5%, 78.3%, 60.6%, 48.5%, and 28.3% of flood pixels within 54.7%, 42.2%, 30.5%, 27.0%, and 25.1% of the total area, respectively. The RF models achieved area under the curve (AUC) values exceeding 0.850, with a maximum of 0.966. Furthermore, a standard deviation map derived from the RF models identified regions of high and low uncertainty, highlighting areas for potential methodological improvement and targeted sampling. The results also show the promise of the multilevel approach for mapping flood susceptibility and call for more research into its potential for future studies and real-world applications.

How to cite: Gorsevski, P. and Milevski, I.: Multilevel flood susceptibility mapping by fuzzy sets, analytical hierarchy process, weighted linear combination and random forest, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14278, https://doi.org/10.5194/egusphere-egu26-14278, 2026.

Spatial statistics provides a principled framework for analyzing environmental variables that exhibit spatial dependence, enabling inference and prediction in systems governed by heterogeneous processes. In many hydrogeological applications, the most informative perspective emerges from fusing complementary datasets, for example, sparse groundwater observations and spatially exhaustive remote sensing products. This data fusion is rarely straightforward because data sources often differ in sampling design, uncertainty, and, crucially, spatial support (the area or footprint represented by a measurement). When observations collected at one support are used to predict at another, the change-of-support problem can induce biased variances and degraded predictions if scale effects are ignored. Here, we integrate groundwater levels from a monitoring network with multi-resolution remote sensing covariates to improve groundwater depth mapping while explicitly accounting for support differences. The study targets groundwater level prediction in Southeast Brazil, where relief compartments and land-use patterns generate strong spatial heterogeneity in recharge and water consumption. We combine in situ groundwater table depths observed at 56 monitoring locations with (i) geomorphological information derived from the 30 m TanDEM‑X dataset and (ii) land-surface water consumption represented by 10 m evapotranspiration estimates from SAFER (Simple Algorithm for Evapotranspiration Retrieving). These covariates encode terrain-driven controls and land-use effects that are not fully captured by point measurements alone. Spatial dependence within and across variables is modeled using the Linear Model of Coregionalization (LMC), enabling coherent estimation of direct and cross-variograms. To ensure consistency across supports, we address support homogenization by regularizing point-support variances and cross-structures to a common block support defined on the prediction grid. This regularized LMC is then used within a collocated block cokriging (CBCK) framework, which applies collocated block covariates to enhance block-scale groundwater predictions. Model performance demonstrates substantial gains from explicitly treating change of support and incorporating multi-resolution covariates. CBCK yields reliable groundwater depth predictions with root mean squared error (RMSE) of 0.41 m, markedly outperforming ordinary block kriging (OBK) estimations (RMSE = 2.89 m) and improving upon prior CBCK implementations that relied on coarser (500 m) evapotranspiration inputs (RMSE = 0.49 m). Beyond accuracy improvements, the resulting maps better reflect the coupling between land-use water demand, terrain-driven controls, and groundwater levels, supporting groundwater management decisions relevant to agronomic planning and ecosystem sustainability. The proposed methodology is transferable to other aquifer systems and can be adapted to alternative remote sensing products and field measurements to explore climate, land use, and hydrogeology interactions across spatial scales.

How to cite: Lilla Manzione, R. and de Oliveira Ferreira Silva, C.: Multi-source data fusion to enhance groundwater levels prediction: merging monitoring networks and orbital remote sensing datasets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22108, https://doi.org/10.5194/egusphere-egu26-22108, 2026.

EGU26-2847 | Posters on site | EOS2.4

Validating Research Data Management Core Competencies: A survey of US data librarianship current practices to inform the curricula 

Wade Bishop, Angela Murillo, Ayoung Yoon, and Alex Chassanoff

In the context of massive datasets across disciplines, US higher education institutions provide research data services in their academic libraries and elsewhere on campuses. The core competencies to perform these emerging occupations have been developed through an extensive literature review and focus groups. This presentation will provide results from a survey validation study of current professionals to validate core competencies for research data management (RDM). The sampling frame is of data managers, stewards, curators and any related professionals from a variety of communities including, Academic Research Library (ARL) institutions, International Association for Social Science Information Service and Technology (IASIST), Research Data Alliance (RDA), Committee on Data (CODATA), Research Data Access and Preservation Association (RDAP), Earth Science Information Partners (ESIP), and others. Although US-focused, the survey findings can help determine the most important core competencies to include in any RDM curricula. The curricula resulting from the survey validation is delivered in US information schools (iSchools), but lessons learned could be used to inform curricula in any domain and address the gap in earth and environmental science education.

How to cite: Bishop, W., Murillo, A., Yoon, A., and Chassanoff, A.: Validating Research Data Management Core Competencies: A survey of US data librarianship current practices to inform the curricula, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2847, https://doi.org/10.5194/egusphere-egu26-2847, 2026.

Each summer, the Institute for Geospatial Understanding through an Integrative Discovery Environment (I-GUIDE) project, funded by NSF’s Harnessing the Data Revolution initiative, organizes a Summer School. I-GUIDE’s vision is to “Drive digital discovery and innovation by harnessing the geospatial data revolution.”

 

The I-GUIDE Summer School is a gathering of graduate students, post-doctoral researchers and early career scholars who go on a week-long intellectual journey. The Summer School is not just an event; it's a convergence of minds, ideas, and cutting-edge methodologies to shape the future of geospatial understanding.  The Summer School champions the spirit of Geospatial Convergence Science, leveraging AI, and it is rooted in the belief that some of the most pressing societal challenges demand a collaborative, multidisciplinary approach.

 

I-GUIDE has thus far conducted three highly successful Summer Schools with themes Convergence Science in Action, Leveraging AI for Environmental Sustainability, and Spatial AI for Extreme Events and Disaster Resilience. The three Summer Schools were held at the University Corporation for Atmospheric Research facilities in Boulder, CO, and they share a few common key features:

 

  • Convergence Science in Action: Participants navigate the intersection of various disciplines, strategically integrating knowledge, tools, and modes of thinking. The program emphasizes collaborative and professional interactions, fostering an environment where participants learn to work comprehensively on convergence science problems.
  • Interactive Learning: Participants engage in a week-long immersive experience, collaborating with I-GUIDE members to develop novel solutions to computation- or data-intensive geospatial data science challenges. They delve into geoethics, geo-enabling reproducible and open science, geovisualization, and the latest in geoAI via cloud and high-performance computing.
  • Diverse Application Areas: Each year, the participants address critical topics such as climate change, biodiversity, water security, sustainable development, changes in wildland-urban interface, social science data and ethical implications.
  • Integration of Ethics: Ethical considerations, including Collection Bias and Limitations, Missing Perspectives, Assumption of Homogeneity, and Unintended uses.
  • Independent External Evaluation: Conduct surveys, focus group interviews, and use other evaluation tools to capture participant feedback to improve learning outcomes through continuous evaluation and refinement.
  • Ongoing Engagement: Participants continue to stay engaged with the I-GUIDE project by participating in various events and activities, including attending and presenting at the I-GUIDE forum and giving talks to the broader community via the Virtual Consulting Office.

 

In this presentation, we will provide an overview of the Summer Schools, along with relevant highlights, key outcomes, and the lessons learned. We will discuss the geospatial, computational and AI/machine learning, and collaborative working skills the participants learn and apply to work on the projects, along with the incentives I-GUIDE provides for the participants’ success.

How to cite: Ramamurthy, M.: The I-GUIDE Summer School: An annual learning experience that promotes geospatial convergence science and AI to tackle complex scientific and societal challenges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8543, https://doi.org/10.5194/egusphere-egu26-8543, 2026.

EGU26-12247 | Posters on site | EOS2.4 | Highlight

Building Foundational Climate Data Skills Through Hands-On Training with ESA-CCI's Essential Climate Variables 

Amina Maroini, Lisa Beck, Sarah Connors, Tonio Fincke, and Eduardo Pechorro

Understanding climate change relies on sustained observations of Essential Climate Variables (ECVs), as defined by the Global Climate Observing System (GCOS). As access to ECVs has expanded in scope and duration, users are increasingly confronted with the complexity of these datasets, including longer time series, different data structures, multiple product versions, and uncertainty estimates. 

To remove common technical barriers, such as installing software and coding libraries or, locating and downloading large datasets, the European Space Agency’s Climate Change Initiative (ESA-CCI) developed a cloud-based, pre-configured JupyterLab environment designed to allow learners to begin working with satellite-derived ESA-CCI climate data within minutes.  

This pre-configured JupyterLab environment supports users by integrating simplified access to decades-long global records of the 27 satellite-derived ESA-CCI ECVs into the ESA CCI Toolbox, a dedicated Python package specifically designed for ESA-CCI data that provides ready-to-use functions, allowing users to focus on visualising and analysing climate signals rather than writing custom code from scratch. 

We present this environment as the foundation for a series of training events that have successfully engaged diverse audiences, including students, early-career researchers, and non-specialist stakeholders1. Through guided notebooks that walk learners  through accessing ESA-CCI data, filtering and aggregating variables, visualising spatial and temporal patterns, and exploring uncertainties and data quality flags, learners gain hands-on, reproducible climate data analysis experience while deepening their understanding of the significance of satellite-derived ECVs and their role in monitoring and interpreting climate change. Our presentation will give the opportunity for conference participants to explore the JupyterLab environment during the PICO session. 

1 https://climate.esa.int/en/climate-change-initiative-training/training-sessions/ 

How to cite: Maroini, A., Beck, L., Connors, S., Fincke, T., and Pechorro, E.: Building Foundational Climate Data Skills Through Hands-On Training with ESA-CCI's Essential Climate Variables, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12247, https://doi.org/10.5194/egusphere-egu26-12247, 2026.

EGU26-12625 | ECS | Posters on site | EOS2.4

Improving the Usability and Adoption of Digital Data Solutions: An Example for Researchers in the Digital Waters Flagship and PhD Pilot  

Mohammad Imangholiloo, Elizabeth Carter, and Ville Mäkinen

Geospatial data are increasingly available openly online, and often they are accessible in multiple ways, including web application programming interfaces (API) by the Open Geospatial Consortium (OGC). However, researchers often continue to rely primarily on manually downloading datasets to their laptops for their daily research activities. This workflow has some disadvantages. For example, if the input data updates often, making sure that all the researchers working on the topic have the exact same dataset available is a manual and an error-prone process. The use of web APIs could provide help for various use cases but requires some IT knowledge that many substance experts may lack. 

To address this challenge, we developed a set of Jupyter Notebook examples designed to support researchers in accessing, exploring, and analyzing geospatial data from APIs in both virtual and local computing environments. The notebooks demonstrate and compare multiple approaches for directly accessing vector, raster, and point cloud data, as well as associated metadata records. We test the notebooks on a course for PhD students related to the Digital Waters Flagship by the Research Council of Finland and evaluate their effectiveness using a questionnaire for the course participants.  

With the proposed approach, we aim to lower technical barriers and facilitate the integration of distributed data into existing research workflows. Ultimately, these practices can support the creation of digital twins of water resources and contribute to intelligent and sustainable water management. 

 

Keywords: geospatial data, data infrastructures, Jupyter notebook, data space, technical barriers 

How to cite: Imangholiloo, M., Carter, E., and Mäkinen, V.: Improving the Usability and Adoption of Digital Data Solutions: An Example for Researchers in the Digital Waters Flagship and PhD Pilot , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12625, https://doi.org/10.5194/egusphere-egu26-12625, 2026.

EGU26-14682 | Posters on site | EOS2.4

Motivations, goals and design of new interdisciplinary Computer Science and Geology degrees at the bachelor’s and master’s levels 

Elizabeth H. Madden, Kimberly Blisniuk, Emmanuel Gabet, and Genya Ishigaki

Today’s geoscience challenges and opportunities, such as those associated with environmental health, energy production, mineral extraction, fresh water and natural hazards, demand that public employees, private sector workers and researchers have skills across the fields of geology, geophysics and computer science. In addition, the integration of computing methods into global culture underscores the need to train professionals that ask key questions and make informed decisions about their best uses. In the context of geosciences, it is critical that people with an understanding of the science manage how computing methods are used to select, store, analyze and organize data, create digital public interfaces, and run models. While challenging, this provides opportunities to expand and renew geoscience education in order to promote its relevance into the future. In light of this, San José State University (SJSU) in San José, California USA, is launching a new bachelor’s degree titled ‘Computer Science and Geology’ and a new master’s degree titled ‘Computational Geoscience’ aimed at training students in both geoscience topics and computer science skills. 

We have designed these programs to provide an integrated educational experience in quantitative methods, computer programming and the gathering, analysis, storage and sustainable management of large environmental, geological, and geophysical data sets. The degrees at both educational levels include an array of courses and broad faculty expertise in the separate departments of Computer Science and Geology at SJSU in data analysis, machine learning, artificial intelligence, geological and geophysical modeling across a range of geoscience topics, and natural hazards assessment. These degrees aim to equip students with applied skills to meet a growing workforce demand, and also ensure that this workforce recognizes the possibilities, limitations and dangers of computing tools and methods. The presence of SJSU in the heart of Silicon Valley, SJSU’s role in the U.S. university system as a primarily undergraduate serving institution, and the success of SJSU at transforming students’ lives through career advancement make this a positive place to launch these interdisciplinary degree programs. Through this presentation, we also hope to learn more about best practices and challenges of initiatives and programs at other universities to help guide the development of these degrees and best meet the needs of students and the future research, public service and private sector workforces.

How to cite: Madden, E. H., Blisniuk, K., Gabet, E., and Ishigaki, G.: Motivations, goals and design of new interdisciplinary Computer Science and Geology degrees at the bachelor’s and master’s levels, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14682, https://doi.org/10.5194/egusphere-egu26-14682, 2026.

EGU26-16396 | ECS | Posters on site | EOS2.4

Co-developing research-assisting AI for water resources professionals: the Digital Waters Flagship’s digital methods course  

Elizabeth Carter, Mehrdad Rostami, Elsa Culler, Omer Abubaker, Mohammad Imangholiloo, Mia Pihlajamäki, Maija Taka, Harri Koivusalo, Pertti Alo-Aho, Hannu Martilla, Mehdi Rasti, Pyry Kettunen, Marko Keskinen, Ville Mäkinen, Juha Oksanen, Petteri Alho, and Björn Klöve

The accelerating complexity of global water challenges—driven by hydrologic intensification, a growing and urbanizing population, and proliferation of observational data—demands a new generation of water‑domain researchers who are both computationally fluent and capable of critically integrating artificial intelligence (AI) into scientific workflows. Yet, most geoscience doctoral programs provide limited training in open, reproducible computational methods, and generic AI tools often underperform in specialized environmental domains while lacking transparent attribution of sources. To address these gaps, the Digital Waters Flagship initiative designed and implemented an innovative doctoral‑level course that integrates open‑science software training with student‑driven co‑development of a domain‑adapted large‑language model (LLM) for hydrologic research assistance.

The course employs a flipped‑classroom model within the Digital Waters Virtual Research Environment (VRE), where students learn standardized, reproducible workflows using a repository structure composed of six core elements spanning data access, processing, modeling, visualization, and computational environments. Exceptional student repositories are publicly disseminated as open digital water use cases. In parallel, doctoral researchers participate in the co‑design of a hydrology‑focused research chatbot, DIWA ReChat, which is trained on authentic student‑generated workflow components and equipped with automatic knowledge‑source attribution to ensure transparency and proper crediting of contributions.

Course outcomes are evaluated through (1) pre‑/post‑assessment of computational competency, (2) evidence of improved reproducibility enabled by shared VRE infrastructure, and (3) empirical improvements in domain‑adapted LLM performance based on both conventional accuracy metrics and student‑designed AI efficacy criteria. Together, the course and chatbot development process demonstrate a scalable model for integrating open‑science education with responsible, domain‑aware AI tool creation. This work highlights a pathway for cultivating computationally capable researchers who can both leverage and critically evaluate AI in support of robust, transparent hydrologic science.

How to cite: Carter, E., Rostami, M., Culler, E., Abubaker, O., Imangholiloo, M., Pihlajamäki, M., Taka, M., Koivusalo, H., Alo-Aho, P., Martilla, H., Rasti, M., Kettunen, P., Keskinen, M., Mäkinen, V., Oksanen, J., Alho, P., and Klöve, B.: Co-developing research-assisting AI for water resources professionals: the Digital Waters Flagship’s digital methods course , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16396, https://doi.org/10.5194/egusphere-egu26-16396, 2026.

EGU26-19756 | Posters on site | EOS2.4

Introduction to Python for Geographic Data Analysis: A new, open resource for teachers and learners 

David Whipp, Henrikki Tenkanen, and Vuokko Heikinheimo

Digital geoscientific and geospatial datasets are rapidly growing in both number and size. These data present powerful new resources for understanding the evolution of the earth, but working with them requires computational skills are not part of typical geoscience curricula at universities. To leverage the power of these growing geoscientific and geospatial data, students need targeted educational resources that provide basic computational skills.

The new textbook Introduction to Python for Geographic Data Analysis provides a framework for learning to work with (geospatial) datasets of varying size from loading the data to producing interactive visualizations of processed data. Part 1 of the book covers the basics of programming using the Python language, introducing both programming concepts and their Python syntax. It also covers the analysis of tabular data using the pandas Python library and the basics of data visualization. Part 2 introduces working with geospatial data, including fundamental geospatial concepts, working with vector and raster data, geospatial data visualization, and loading data from online sources. Part 3 includes several case studies that build on things presented in the first two parts to demonstrate what can be done with the readers’ new skills. Finally, the appendices provide information about best practices in programing, version control with git and GitHub, and other practical coding tips that promote open, reproducible science.

The book materials are freely available online at https://pythongis.org, and we anticipate that hard copies of the book will be available later in 2026. We hope the book will appeal to a broad range of “geo” scientists, including teachers who provide courses on introductory programming or data analysis for geology and geography students, those interested in learning to interact with and batch process large datasets, and those interested in finding open-source alternatives to commercial GIS software packages.

How to cite: Whipp, D., Tenkanen, H., and Heikinheimo, V.: Introduction to Python for Geographic Data Analysis: A new, open resource for teachers and learners, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19756, https://doi.org/10.5194/egusphere-egu26-19756, 2026.

EGU26-20494 | ECS | Posters on site | EOS2.4

Textbook and code: AI for climate scientists 

Simon Driscoll, Kieran Hunt, Laura Mansfield, Ranjini Swaminathan, Hong Wei, Eviatar Bach, and Alison Peard

We introduce a textbook for climate modellers and scientists seeking to learn AI.

Weather and Climate: Applications of Machine Learning and Artificial Intelligence provides a comprehensive exploration of machine learning in the context of weather forecasting and climate research. The authors begin with an introduction to the fundamentals and statistical tools of machine learning, followed by an overview of various machine learning models. Emulation and machine learning of sub-grid scale parametrizations are discussed, along with the application of AI/ML in weather forecasting and climate models. Next, the book delves into the concept of explainable AI (XAI) methods for understanding ML and AI models, as well as the use of generative AI in weather and climate research. It explores the interface of data assimilation and machine learning for weather forecasting, showcasing case studies of machine learning applied to environmental monitoring data. The book concludes by looking ahead to the future of ML and AI in climate and weather-related research, providing references for further reading. This comprehensive guide offers valuable insights into the intersection of machine learning, artificial intelligence, and atmospheric science, highlighting the potential for innovation and advancement in weather and climate research.

How to cite: Driscoll, S., Hunt, K., Mansfield, L., Swaminathan, R., Wei, H., Bach, E., and Peard, A.: Textbook and code: AI for climate scientists, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20494, https://doi.org/10.5194/egusphere-egu26-20494, 2026.

EGU26-1499 | ECS | Posters on site | ESSI3.4

Navigating legacy Earth System Model software 

Lakshmi Aparna Devulapalli

As a Research Software Engineer in the natESM project, you have the opportunity to work with a wide range of Earth System Models (ESMs) developed by the German scientific community. Many of these models, originating in the 1990s, were predominantly written in Fortran. While the broader scientific software world has since transitioned toward languages such as C/C++ and Python, the ESM community is still in the process of catching up. As a result, legacy Fortran code—often 20 years old or more—presents unique and sometimes amusing challenges when attempting to adapt or port to modern technologies.

This talk offers a humorous look at these challenges through the eyes of an RSE navigating outdated code in order to accomplish present-day tasks. Topics will include unsustainable methods of structuring software, relic configuration files used for input, ambiguous naming conventions, unused or nonfunctional code that has never been removed, version control practices that can be improved, and other long-standing programming habits that need to evolve. The session will also highlight more modern and maintainable alternatives to these practices, offering a lighthearted yet constructive perspective on bringing legacy ESM code into the future.

How to cite: Devulapalli, L. A.: Navigating legacy Earth System Model software, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1499, https://doi.org/10.5194/egusphere-egu26-1499, 2026.

natESM is a project that brings together German resources to develop a seamless, multiscale Earth System Modelling framework that can serve multiple purposes. This system is composed of several independent and diverse software models from the community, each addressing different parts of the Earth system. Given the variety of programming languages, model sizes and software architectures involved, as well as different experience among the responsible model developers, challenges arise in portability, performance and software quality. 

A key part of the natESM approach is the technical support to model developers provided by Research Software Engineers (RSEs). Their work focuses not only on integration, portability and performance, but also on systematically improving software quality within and across model components. This talk will outline the progress made so far, highlight lessons learned from the RSE-scientist collaborations, and present our future plans for assessing and enhancing software quality. The experiences and methods developed in natESM might serve as an example for improving software sustainability in Earth System Modeling more broadly.

How to cite: Loch, W. J.: The natESM Journey for Improving Software Quality in Earth System Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1645, https://doi.org/10.5194/egusphere-egu26-1645, 2026.

Scientific software often begins as an internal research tool developed by scientists rather than trained software engineers, resulting in limited usability, documentation, and maintainability. emiproc, a tool for processing emission inventories for atmospheric chemistry and transport models, originally followed this trajectory: it grew organically within our laboratory, offered only a command-line interface, and lacked a clear structure, extensibility, and user-oriented documentation. We recently undertook a full modernization of emiproc following the best practices in scientific software development: redesign of the code base into modular components, consistent object oriented Python API, automated testing with continuous integration, extensive documentation for both users and developers and publication in the Journal of Open Source Software. The updated software now supports some of the most widely used emission inventories such as EDGAR and CAMS, and more specific ones like the City of Zurich inventory, and produces output for various transport models like ICON-ART, WRF, or GRAL. We will highlight our approaches for transforming emiproc into a sustainable and user-friendly tool and reflect on the challenges we encountered along the way. By sharing our experience, we aim both to contribute to the discussion on improving scientific software development and to learn from the approaches used by others. 

How to cite: Constantin, L. and Brunner, D.: Scientific Software Developement: Lessons from our Emission inventory processing software emiproc  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3484, https://doi.org/10.5194/egusphere-egu26-3484, 2026.

Geochemistry π is an open-source automated machine learning Python framework. Geochemists need only provide tabulated data (e.g. excel spreadsheet) and select the desired options to clean data and run machine learning algorithms. The process operates in a question-and-answering format, and thus does not require that users have coding experience. Version 0.7.0 includes machine learning algorithms for regression, classification, clustering, dimension reduction and anomaly detection. After either automatic or manual parameter tuning, the automated Python framework provides users with performance and prediction results for the trained machine learning model. Based on the scikit-learn library, Geochemistry π has established a customized automated process for implementing machine learning. The Python framework enables extensibility and portability by constructing a hierarchical pipeline architecture that separates data transmission from algorithm application. The AutoML module is constructed using the Cost-Frugal Optimization and Blended Search Strategy hyperparameter search methods from the A Fast and Lightweight AutoML Library, and the model parameter optimization process is accelerated by the Ray distributed computing framework. The MLflow library is integrated into machine learning lifecycle management, which allows users to compare multiple trained models at different scales and manage the data and diagrams generated. In addition, the front-end and back-end frameworks are separated to build the web portal, which demonstrates the machine learning model and data science workflow through a user-friendly web interface. In summary, Geochemistry π provides a Python framework for users and developers to accelerate their data mining efficiency with both online and offline operation options. All source code is available on GitHub  (https://github.com/ZJUEarthData/geochemistrypi), with a detailed operational manual catering to both users and developers (https://geochemistrypi.readthedocs.io/en/latest/).

How to cite: ZhangZhou, J. Z.: Geochemistry π: Machine Learning for Geochemists Who Don’t Want to Code, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5192, https://doi.org/10.5194/egusphere-egu26-5192, 2026.

 

Advances in computing, statistics, and machine learning (ML) techniques have significantly changed research practices across disciplines. Despite Fortran’s continued importance in scientific computing and long history in data-driven prediction, its statistics and ML ecosystem remains thin. FSML (Fortran Statistics and Machine Learning) is developed to address this gap and make data-driven research with Fortran more accessible. 

The following points are considered carefully in its development and each come with their own challenges, solutions, and successes: 

  • Good sustainable software development practices: FSML is developed openly, conforms to language standards and paradigms, uses a consistent coding and comment style, and includes examples, tests, and documentation. A contributor’s guide ensures consistency for future contributions. 
  • Accessibility: FSML keeps the code clean and simple, avoids overengineering, and has minimal requirements. Additionally, an example-rich html documentation and tutorials are automatically generated with the FORtran Documenter (FORD) from code, comments, and simple markdown documents. Furthermore, it is developed to support compilation with LFortran (in addition to GFortran), so it can be used interactively like popular packages for interpreted languages. 
  • Community: FSML integrates community efforts and feedback. It uses the linear algebra interfaces of Fortran’s new de-facto standard library (stdlib) and the fortran package manager (fpm) for easy building and distribution. Its permissive licence (MIT) allows developers to integrate FSML into their projects without the restrictions often imposed by other licenses. Its simplicity, documentation, contributor’s guide, and GitHub templates remove barriers for new contributors and users. 
  • Communication: FSML updates are shared through a variety of methods with different communities. This includes a journal article (https://doi.org/10.21105/joss.09058) for visibility among academic colleagues, frequently updated online documentation (https://fsml.mutz.science/), social media updates, as well as a blog and Fortran Discourse posts to keep Fortran’s new and thriving online community updated. 

Early successes of FMSL’s approach and design include: 1) Students with little coding experience were able to learn the language and use library with only Fortran-lang’s tutorials and FSML’s documentation; 2) early career researchers with no prior experience in Fortran used FSML’s functions to conduct research for predicting future climate extremes; 3) FSML gained a new contributor and received a pull request only days after its first publicised release. 

The development of FSML demonstrates the merits of using good and open software development practices for academic software, as well as the potential of using the new Fortran development ecosystem and building bridges to the wider (non-academic) developer community. 

How to cite: Mutz, S. G.: Developing a modern Fortran statistics and machine learning library (FSML) , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5393, https://doi.org/10.5194/egusphere-egu26-5393, 2026.

EGU26-6222 | ECS | Posters on site | ESSI3.4

Preparing for an Operational Environment: Software Development Standards in the Integrated Greenhouse Gas Monitoring System for Germany 

Diego Jiménez de la Cuesta Otero and Andrea Kaiser-Weiss

Modern scientific projects typically rely on software, e.g., for implementing numerical models, performing data pre- and postprocessing, solving inverse problems, or assimilating observations. Consequently, the reliability and reproducibility of scientific results critically depend on software quality. Scientific results are also intended to be shared or reused, and so is the software that produces them: especially in operational settings, where traceability and maintainability are essential. Therefore, a sustainable software development strategy becomes key to a project's success. Nevertheless, often software standards are treated as a secondary concern. This can lead to difficulties when introducing new features, delays in users' projects, limited reproducibility, strained collaborations, and ultimately lack of suitability for operational use.
 
We present the case of the German Weather Service (DWD) contributions within the Integrated Greenhouse Gas Monitoring System for Germany (ITMS). The primary objective of ITMS is the verification of greenhouse gas emissions, which imposes particularly high requirements on the results' traceability and reproducibility. Accordingly, most if not all software-based components of our system should adhere to software development standards that ensure these requirements. We provide an overview of our software development standards and their application, and discuss lessons learned that are transferable to both legacy and newly developed scientific software projects.

How to cite: Jiménez de la Cuesta Otero, D. and Kaiser-Weiss, A.: Preparing for an Operational Environment: Software Development Standards in the Integrated Greenhouse Gas Monitoring System for Germany, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6222, https://doi.org/10.5194/egusphere-egu26-6222, 2026.

EGU26-7565 | Orals | ESSI3.4

The Modular Earth Submodel System (MESSy): lessons learned from 20+ years of continuous development 

Patrick Jöckel, Astrid Kerkweg, Kerstin Hartung, and Bastian Kern

Earth System Models (ESMs) aim at replicating the essence of the Earth Climate System in numerical simulations on high performance computing (HPC) systems. The underlying software is often rather complex, comprising several source code entities (modules and libraries, sometimes combining different programming languages), and has in many cases grown over decades. ESMs are usually structured as “multi-compartment” models, i.e. disassembled into a set of different components, each of which describes a different compartment in the Earth System, such as the atmosphere, the land surface, the ocean, the cryosphere, the biosphere, etc. Each compartment model, in turn, comprises a series of algorithms (numerical solvers, parametrizations), each of which represents a specific physical, chemical or socio-economic process. The behaviour of the “system as a whole” (i.e., the development of its state over time, its response to perturbations) is characterized by non-linear interactions and feedbacks between the different compartments and processes.

The implementation of such numerical models representing these inter-compartment and inter-process connections (i.e. the coupling) poses a challenging task for the software development, in particular given the need for (scalable) continuous further development and integration of new components, aiming at keeping pace with our knowledge about the real Earth System. Common requirements to such software are maintainability, sustainability (e.g. for new HPC architectures), resource efficiency (performance at run-time), but also development scalability.

More than twenty years ago (in 2005) we proposed the Modular Earth Submodel System (MESSy) as a potential new approach to Earth System modelling. Here, we present how we started as an “atmospheric chemistry add-on” to a specific General Circulation Model, but already with a wider range of applications in mind. We further show, how we went through our 2nd development cycle, finally arriving at our current state, the MESSy Integrated Framework that is soon to be released Open Source. Although our 4 major software design principles (will be presented!) did not change significantly from the early stage, we had to undergo several implementation revisions to reach its current state. Despite the continuous development, MESSy was always “state-of-the art” and “in operation”, i.e. used for scientific research. Thus, in retrospect, we present some of the milestones achieved by “pragmatic” software engineering in practice.

How to cite: Jöckel, P., Kerkweg, A., Hartung, K., and Kern, B.: The Modular Earth Submodel System (MESSy): lessons learned from 20+ years of continuous development, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7565, https://doi.org/10.5194/egusphere-egu26-7565, 2026.

EGU26-7637 | Posters on site | ESSI3.4

Insights and tips for maintainability, robustness, usability, and reproducibility of geo-scientific models 

Konstantin Gregor, Benjamin Meyer, Joao Darela-Filho, and Anja Rammig

The complexity of geoscientific models, from pre-processing, model execution, and post-processing, poses major challenges to maintainability, reproducibility, and accessibility, even when FAIR data principles are followed.

Based on a survey of the 20 dynamic global vegetation models participating in the Global Carbon Project, we present the current state of, and potential improvements in, practices of software engineering and reproducibility within the community.
We also share notable successful practices from the community that could be helpful for all geo-scientists, including
- version control
- workflow management systems
- containerization
- automated documentation
- continuous integration
- automated visualizations

These approaches enable reproducible, portable, and automated workflows, improve code reliability, and enhance access to scientific results.

We conclude with a showcase of a fully reproducible and portable workflow implemented for one model, illustrating how these practices can be implemented by other modeling communities. This example can serve as a practical resource for improving reproducibility, accessibility, and software engineering standards across the geosciences.

How to cite: Gregor, K., Meyer, B., Darela-Filho, J., and Rammig, A.: Insights and tips for maintainability, robustness, usability, and reproducibility of geo-scientific models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7637, https://doi.org/10.5194/egusphere-egu26-7637, 2026.

EGU26-8659 | Orals | ESSI3.4

Improving long-term maintainability of the ACCESS models while transitioning to new architectures: challenges and opportunities 

Micael J. T. Oliveira, Edward Yang, Manodeep Sinha, and Kelsey Druken

Australia’s Climate Simulator, ACCESS-NRI, is Australia’s National Research Infrastructure (NRI) for climate modelling, supporting the development and community use of the Australian Community Climate and Earth System Simulator (ACCESS). 

As the ACCESS modelling system evolves to meet user requirements, so does the basic infrastructure that underpins our ability to efficiently run the models, with HPC architectures rapidly shifting towards GPUs, and new developments in Machine Learning disrupting how new models are developed and used. Under such circumstances, it's easy for scientists and software engineers to focus on more pressing matters and spend less time worrying about software maintainability. Although such type of "tactical" programming might bring benefits in the short term, long-term software maintainability and sustainability requires a more strategic approach. 

Using ACCESS-NRI as a case study, this presentation argues that addressing these challenges is not about any single tool or practice, but about adopting an integrated and coordinated strategy for scientific software development. I will describe how ACCESS-NRI is tackling these challenges by bridging skills and training gaps between scientists and software engineers, adopting well-established industry standards where appropriate (e.g. CMake, Git), and embedding software engineering best practices across development workflows. Alongside these technical efforts, addressing the social challenges of collaboratively developing large, open-source software is a key part of our approach, ensuring contributors can work effectively towards shared goals. 

A concrete example is GPU porting within the ACCESS modelling system. Successfully porting code to GPUs has required close collaboration with existing code owners, careful consideration of scientific and performance constraints, and a strong emphasis on avoiding divergent code paths that are difficult to maintain. This experience highlights the importance of the social dimensions of software development: changes cannot simply be imposed, but must be developed collaboratively to balance reliability, performance, portability, and long-term sustainability. 

By reflecting on what has worked—and what has not—this talk aims to share practical lessons that are transferable to other scientific software projects as they grow beyond small research teams into widely used, community-supported systems.

How to cite: Oliveira, M. J. T., Yang, E., Sinha, M., and Druken, K.: Improving long-term maintainability of the ACCESS models while transitioning to new architectures: challenges and opportunities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8659, https://doi.org/10.5194/egusphere-egu26-8659, 2026.

EGU26-8712 | Orals | ESSI3.4

 Modern tools to scale the compilation, testing and deployment of scientific software  

Aidan Heerdegen, Tommy Gatti, Harshula Jayasuriya, Thomas McAdam, Johanna Basevi, and Kelsey Druken

Modern software development practices such as continuous integration compilation, testing and deployment are a requirement for robust and trusted climate model development. However, this can be very challenging to achieve with climate models that often include legacy code requiring very specific versions of scientific libraries and that must run on complex HPC systems.  In addition, climate models have very long support timeframes (5+ years), with a requirement for absolute bitwise reproducibility, which requires precise control and provenance of the entire software stack. 

Australia’s Climate Simulator (ACCESS-NRI), is a national research infrastructure tasked with supporting the development and use of the Australian Community Climate and Earth System Simulator (ACCESS) model suite for the research community. At ACCESS-NRI we use spack, a build from source package manager targeting HPC, to create infrastructure to easily build ACCESS climate models and their supporting software stacks with full provenance and build reproducibility.  

Now the challenge for us at ACCESS-NRI, as an infrastructure supporting a wide range of user needs, is to scale this effort to multiple models, with many permutations of components and versions, without creating a very large support burden for our software engineers.  

We do this by focusing on modularity and generic workflows to achieve our desired scale efficiently. Spack's modular design has meant ACCESS-NRI has been able to create entirely generic GitHub workflows for building, testing and deploying many climate models on our target HPC, Australia’s National Computational Infrastructure (NCI), as well as run test builds on standard Linux virtual machines.  

As a result there is dramatically less support burden, as the CI/CD code is centralised and maintained in one location, and reused in many places. It is also extremely simple to add CI testing for new model components with just a few lines of GitHub Actions code. 

The choice of tools allowing a focus on a modular approach and generic workflows has been validated: we currently support seven models, with nineteen discrete components, and have grown from one deployment in 2023, eleven in 2024 and now twenty-nine in 2025,  as well as many thousands of pre-release test builds in the last quarter alone. This gives us confidence that we can continue to scale efficiently, without a large support burden requiring onerous resourcing that might otherwise place a technical limit on future activities. 

How to cite: Heerdegen, A., Gatti, T., Jayasuriya, H., McAdam, T., Basevi, J., and Druken, K.:  Modern tools to scale the compilation, testing and deployment of scientific software , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8712, https://doi.org/10.5194/egusphere-egu26-8712, 2026.

EGU26-9441 | Posters on site | ESSI3.4

The Data-to-Knowledge Package - A Framework for publishing reproducible and reusable analysis workflows in Earth System Science 

Markus Konkol, Simon Jirka, Sami Domisch, Merret Buurman, Vanessa Bremerich, and Astra Labuce

More and more funders, reviewers, and publishers ask researchers to follow Open Science principles and make their research results publicly accessible. In the case of a computational analysis workflow, this means providing access to data and code that produced the figures, tables, and numbers reported in a paper. However, doing so, even in consideration of the FAIR Principles, does not mean others can easily reuse the materials and continue the research. It still requires effort to understand an analysis script (e.g., written in R or python) and extract those parts of a workflow (i.e. the code snippets) that generate, for instance, a particular figure.

In this contribution, we demonstrate the concept and realization of the Data-to-Knowledge Package (D2K-Package), a collection of digital assets which facilitate the reuse of computational research results [1]. The heart of a D2K-Package is the reproducible basis composed of the data and code underlying, for instance, a statistical analysis. Instead of simply providing access to the analysis script as a whole, the idea is to structure the code into self-contained and containerized functions making the workflow steps more reusable. Each function follows the input-processing-output-logic and fulfills a certain task such as data processing, analysis, or visualization. Creating such a reproducible basis allows inferring the following components that are also part of the D2K-Package:

A virtual lab is a web application, for example, in the form of a JupyterLab environment provided with the help of MyBinder. Users can access it via the browser and obtain a computational environment with all dependencies and the runtime pre-installed. Creating such a virtual lab is possible since all code is containerized and the image is built based on a specification of the used libraries, runtime, and their versions. A virtual lab can help users with programming expertise to engage with the code in a ready-to-use programming environment.

A web API service exposes the encapsulated and self-contained functions such that every function has a dedicated URL endpoint. Users can send requests from their analysis script to that endpoint and obtain the results via HTTP. Hence, they can reuse the functions without copying the code snippets or struggling with dependencies. Such a service can be realized using OGC API Processes and pygeoapi.

The computational workflow connects the functions to an executable analysis pipeline and acts as an entry point to a complex analysis. Such a workflow can help users obtain a better understanding of the functions and relevant input parameters. By using workflow tools such as the Galaxy platform, also users without programming experience receive the chance to change the parameter configuration and see how the new settings affect the final output.

Besides the concepts as outlined above, this contribution will also report on real demonstrators which showcase the idea of a D2K-Package.

This project has received funding from the European Commission’s Horizon Europe Research and Innovation programme. Grant agreement No 101094434.

1) Paper: Konkol et al. (2025) https://doi.org/10.12688/openreseurope.20221.3

How to cite: Konkol, M., Jirka, S., Domisch, S., Buurman, M., Bremerich, V., and Labuce, A.: The Data-to-Knowledge Package - A Framework for publishing reproducible and reusable analysis workflows in Earth System Science, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9441, https://doi.org/10.5194/egusphere-egu26-9441, 2026.

EGU26-10884 | Posters on site | ESSI3.4

Teaming up as domain scientists and research software engineers for a sustainable HELIOS++ scientific software 

Dominic Kempf, Hannah Weiser, Dmitrii Kapitan, and Bernhard Höfle

The Heidelberg LiDAR Operations Simulator (HELIOS) is a scientific software for high-fidelity general-purpose virtual laser scanning (VLS) [1]. Using models for virtual scenes, scanner devices, and platforms, HELIOS allows to reproduce diverse scan scenarios over various geographical environments (forests, cities, mountains) and laser scanning systems (airborne and UAV-borne, mobile, terrestrial). Used for algorithm development, data acquisition planning, and method training for supervised machine learning, HELIOS has been successfully integrated into research workflows across the international laser scanning community.

HELIOS was initially developed in a research-driven environment in Java and released as open-source software [2]. Motivated by growing interest in the scientific community, the codebase was re-implemented in C++ to improve its memory footprint, runtime performance and functionality [3]. Since then, we are actively developing new features. Recent additions include support for dynamic scenes [4], new deflector mechanisms, and plug-ins for other open-source software such as Blender. Considering the continually growing user community, current software development specifically prioritizes quality assurance, reliability, long-term maintainability, and user-friendliness.

Supported by the DFG under the program "Research Software - Quality Assured and Re-usable" [5], the HELIOS++ developer team partnered up with the Scientific Software Center (SSC), a research software engineering service department at Heidelberg University. Combining the expertise of the domain scientist from the HELIOS team and the research software engineers (RSEs) of the SSC, we are strengthening the sustainability and usability of HELIOS. Measures presented in our talk include: Improving testing strategies and Continuous Integration, rewriting the CMake build system, packaging HELIOS as a Conda package, creating standalone installers, introducing a new Python API, and developing new strategies for sharing and reproducing HELIOS simulations. Additionally, we will reflect on the benefits as well as key challenges in fostering fruitful collaborations between domain scientists and RSEs. To this end, we will present as a domain scientist/RSE tandem.

References:

[1] HELIOS++: https://github.com/3dgeo-heidelberg/helios

[2] Bechtold, S., & Höfle, B. (2016): https://doi.org/10.5194/isprs-annals-III-3-161-2016

[3] Winiwarter, L et al. (2022): https://doi.org/10.1016/j.rse.2021.112772

[4] Weiser, H., & Höfle, B. (2026): https://doi.org/10.1111/2041-210x.70189

[5] Project website: https://www.geog.uni-heidelberg.de/en/3dgeo/projects-of-the-3dgeo-research-group/fostering-a-community-driven-and-sustainable-helios-scientific-software

How to cite: Kempf, D., Weiser, H., Kapitan, D., and Höfle, B.: Teaming up as domain scientists and research software engineers for a sustainable HELIOS++ scientific software, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10884, https://doi.org/10.5194/egusphere-egu26-10884, 2026.

EGU26-12310 | Posters on site | ESSI3.4

WRF-Chem-Polar: an open, collaborative, and reproducible framework for modeling the polar atmosphere 

Jennie L. Thomas, Lucas Bastien, Ruth Price, Rémy Lapere, Ian Hough, Erfan Jahangir, Lucas Giboni, and Louis Marelle

Over the past 15 years, substantial developments have been made to adapt the regional chemistry-climate model WRF-Chem for applications in polar environments, with a main focus on the Arctic. These developments address key processes that are either absent from, or insufficiently represented in, the standard WRF-Chem distribution, particularly those controlling aerosol-cloud interactions, boundary layer chemistry, and surface-atmosphere coupling over snow, sea ice, and the polar ocean. However, until now, these advances have been distributed across multiple publications, code branches, and project-specific implementations, limiting transparency, reproducibility, and community use.

Here we present WRF-Chem-Polar, a consolidated and openly available modeling framework that integrates our polar-specific model developments into a single, traceable code base. The framework is hosted on GitHub and is structured around two tightly linked components: (i) a unified WRF-Chem-Polar model code that incorporates developments for polar aerosol and cloud processes and (ii) a dedicated infrastructure for compiling, running, and analyzing simulations.

A key objective of WRF-Chem-Polar (including the model code and infrastructure) is to enable transparent model evolution. All developments are tracked through version control, with automated test cases designed to systematically compare model behavior across code versions. This approach allows scientific changes to be evaluated quantitatively, supports regression testing, and facilitates controlled experimentation when introducing new parameterizations or process representations. The infrastructure also provides transparent workflows for simulation setup, post-processing, and diagnostics, improving reproducibility across users and platforms. Code quality, readability, and consistency is improved via coding style guides and modern software tools that include unit testing and automatic enforcement of linting rules.

By making these developments openly accessible and actively maintained, WRF-Chem-Polar lowers the barrier for the community to apply advanced polar chemistry–aerosol–cloud representations, while providing a robust framework for continued development and evaluation. This effort supports both fundamental process studies and applied research and contributes to broader open-science and FAIR modeling and furthers our objective of uptake of our work within the Earth system modeling community.

How to cite: Thomas, J. L., Bastien, L., Price, R., Lapere, R., Hough, I., Jahangir, E., Giboni, L., and Marelle, L.: WRF-Chem-Polar: an open, collaborative, and reproducible framework for modeling the polar atmosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12310, https://doi.org/10.5194/egusphere-egu26-12310, 2026.

EGU26-13932 | Orals | ESSI3.4

Software as Scientific Infrastructure: CIG’s Role  in Computational Geodynamics and Lessons from Developing ASPECT 

Rene Gassmöller, Wolfgang Bangerth, Juliane Dannberg, Daniel Douglas, Menno Fraters, Anne Glerum, Timo Heister, Lorraine Hwang, Robert Myhill, John Naliboff, Arushi Saxena, and Cedric Thieulot

Modeling software is integral to computational geodynamics, enabling quantitative investigation of planetary mantle, lithosphere and core dynamics across a wide range of spatial and temporal scales. Over the past two decades, the field’s software ecosystem has shifted significantly: codes that were once developed and maintained within single research groups have increasingly evolved into large, modular packages sustained by multi-institutional and often international collaborations. One important factor in this transition has been the establishment of community organizations like the Computational Infrastructure for Geodynamics (CIG), which has provided coordination and shared capacity that individual groups typically cannot sustain on their own.
In this contribution, I highlight benefits and lessons learned from work within CIG and from the development of the geodynamic modeling software ASPECT (Advanced Solver for Planetary Evolution, Convection, and Tectonics). Community organizations can accelerate scientific software development in several ways. Shared infrastructure (project landing pages, established user forums) improves discoverability and supports software adoption by the community. Targeted support, including seed funding, helps projects invest in feature development and maintenance. By streamlining software release and distribution and promoting robust development and testing workflows, community organizations improve software quality and reliability. Training the next generation of computational geoscientists through workshops, tutorials, and user support, builds shared expertise and makes community software more sustainable. Collectively, these activities reduce duplicated effort, lower barriers to entry for new users and contributors, and create pathways for software to evolve in step with scientific and numerical-method advances.
ASPECT provides a concrete example of this community-driven model. Designed to simulate thermal convection with a primary emphasis on Earth’s mantle, it has now been used for a broad range of applications including crustal deformation, magma dynamics, and fluid flow, convection on icy satellites, deformation of the inner core, and digital twins of mineral physics experiments. This widening scope has been possible because ASPECT prioritizes usability and extensibility, to accommodate evolving model complexity, and leverages modern numerical methods such as adaptive mesh refinement and robust linear/nonlinear solvers. From the start, ASPECT has been designed for large-scale parallel simulations required for problems with small-scale features embedded in mantle-scale domains.  It also strategically builds on established external libraries (e.g., deal.II, Trilinos, p4est) rather than re-implementing core algorithms. ASPECT’s success has been enabled by a well-tested framework, extensive documentation, a plugin architecture that simplifies customization, and active encouragement of community contributions through support and recognition. Together, these elements illustrate how organizational infrastructure and software design choices support long-term development and continued methodological innovation in geodynamic modeling, enabling robust simulations that address increasingly complex scientific questions.

How to cite: Gassmöller, R., Bangerth, W., Dannberg, J., Douglas, D., Fraters, M., Glerum, A., Heister, T., Hwang, L., Myhill, R., Naliboff, J., Saxena, A., and Thieulot, C.: Software as Scientific Infrastructure: CIG’s Role  in Computational Geodynamics and Lessons from Developing ASPECT, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13932, https://doi.org/10.5194/egusphere-egu26-13932, 2026.

Process‑based models that explicitly couple soil water and heat transport, canopy radiative transfer, photosynthesis, and surface–atmosphere exchange are increasingly used to connect in‑situ observations with remote‑sensing–relevant land‑surface processes. However, their practical adoption—particularly in heterogeneous urban environments—remains challenging due to complex software dependencies, fragmented preprocessing pipelines, and limited transparency in model configuration. These challenges are exacerbated when such models are accessed through low‑level implementations that are difficult to adapt, reproduce, or extend by domain scientists.

We present rSTEMMUS‑SCOPE, an open‑source R interface to the coupled STEMMUS‑SCOPE modelling framework, designed to apply good practices in scientific software development to a hybrid soil–canopy model that is frequently used by practitioners and researchers interested in ecohydrology, urban climate, and remote sensing. The interface lowers barriers for reproducible experimentation by providing a modular, script‑based workflow that integrates eddy‑covariance forcing, in‑situ soil measurements, vegetation parameters, and multilayer soil discretisation within a transparent R‑based environment that supports from data pre-processing to the visualization of the results.

From a software‑engineering perspective, rSTEMMUS‑SCOPE adopts a modular, script‑based architecture that separates data inputs, model settings, execution, and post‑processing. The package provides reproducible pipelines for preprocessing eddy‑covariance meteorological forcing, precipitation, vegetation parameters, and multilayer soil discretisation (>50 layers), enabling fully scripted end‑to‑end simulations within R. Version‑controlled configuration files, consistent function interfaces, and documented defaults are used to support transparency and extensibility, while example workflows and vignettes lower the entry barrier for users who are domain scientists rather than trained software developers. The design follows a “user‑turned‑developer” paradigm, allowing advanced users to adapt parameterisations and forcing strategies while preserving a stable core interface.

We demonstrate these design choices using an urban case study in a temperate green space in Berlin, where hourly simulations were performed for 2019–2020. Observations from an eddy‑covariance tower and in‑situ soil moisture sensors are used as a software stress test rather than as the primary scientific result. Volumetric soil water content at 60 cm depth was reproduced well (Kling–Gupta Efficiency = 0.82; r = 0.88; α = 1.01), while simulated evapotranspiration captured diurnal and seasonal dynamics (r ≈ 0.67), with systematic biases during low‑energy conditions. Sensitivity experiments illustrate how differences in input data sources and parameter choices propagate through the modelling workflow, highlighting the importance of transparent, reproducible pipelines for diagnosing model behaviour.

We conclude by discussing practical lessons learned in wrapping complex process‑based models in high‑level languages: trade‑offs between modularity and performance, documenting urban‑specific parameter choices without constraining expert use, and testing strategies when upstream physics models are computationally expensive. rSTEMMUS‑SCOPE demonstrates how applying robust software practices enables meaningful, reproducible results and supports early‑career researchers working at the interface of modelling, data, and urban environmental science.

Software availability

rSTEMMUS‑SCOPE (open source): https://github.com/EcoExtreML/rSTEMMUS_SCOPE

How to cite: Duarte Rocha, A. and Aljoumani, B.: rSTEMMUS‑SCOPE: a user‑friendly open‑source R package wrapping a coupled soil–canopy process-based model for urban soil‑moisture and ET — good practices and lessons learned, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15058, https://doi.org/10.5194/egusphere-egu26-15058, 2026.

EGU26-16877 | Orals | ESSI3.4

Beyond Good Practices: Designing Scientific Software for Contribution and Reuse 

Eric Hutton, Gregory Tucker, Mark Piper, and Tian Gan

Lowering the barrier to scientific contribution requires more than adopting good software practices; it requires software structures and standards that make contribution and reuse safe, scoped, and sustainable. We describe how the Community Surface Dynamics Modeling System (CSDMS) addresses these challenges through two complementary efforts: the Landlab modeling framework and the Basic Model Interface (BMI).

Landlab is a Python package designed as a platform for building Earth-surface process models. Over time, we discovered its architecture also promoted the user-turned-developer pathway, which has been critical to its success. While good software practices such as automated testing, continuous integration, documentation, and linting provide a foundation of reliability, Landlab’s component-based architecture has been central to enabling contribution. This design offers contributors clearly scoped and isolated entry points for adding new process models without needing to understand or modify the entire codebase. By enabling contributions from a growing set of domain experts and supporting them through shared maintenance infrastructure, this model expands the pool of invested contributors and reduces reliance on a small number of core developers, strengthening the prospects for long-term project sustainability.

The Basic Model Interface (BMI) complements this approach by providing a lightweight, language-agnostic interface standard that defines how models expose their variables, parameters, and time-stepping controls to the outside world. By separating scientific algorithms from model orchestration, BMI enables models to be reused, coupled, and tested across different frameworks without requiring changes to their internal implementations. Ongoing, community-guided work toward BMI 3.0 aims to extend these capabilities by improving support for parallel execution, clearer state management, and optional interface extensions.

Together, Landlab and BMI illustrate how framework design and community-driven standards can reduce technical debt and enable researchers to contribute reusable and interoperable software without requiring them to become full-time software engineers.

How to cite: Hutton, E., Tucker, G., Piper, M., and Gan, T.: Beyond Good Practices: Designing Scientific Software for Contribution and Reuse, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16877, https://doi.org/10.5194/egusphere-egu26-16877, 2026.

EGU26-17128 | Posters on site | ESSI3.4

A modularized workflow for processing heterogeneous agricultural land use data 

Antonia Degen, Yi-Chen Pao, and Andrea Ackermann

In Germany each federal state is committed to collect required information on funding, farming practices and land use with an “Integrated Administration and Control System” (IACS) (Deutscher Bundestag 2014).

Based on the land parcel identification system (LPIS) as one of the core elements of IACS (European Commission, 2025), georeferenced data along with ancillary data are collected annually since 2005. Mandatory requirements for checks and on-site validations ensure a high data quality which makes IACS data very suitable for research purposes (Leonhardt 2024). Our goal is to create a nation-wide timeseries based on IACS data, that contains detailed information on land use, animal husbandry and farm statistics and can be used for comprehensive land use, soil, agricultural-policy and biodiversity research. Despite this, IACS data remain underused for scientific research due to the following challenges:

  • Data protection: Obtaining and handling IACS data requires a legal agreement between the research project and the respective federal state including Data Usage Agreements.
  • Data heterogeneity: All federal states have unique data processing workflows and historical changes in processing practices resulting in different data-types, -formats, structure, keys, encodings, etc.
  • Data volume: Large storage volume, processing capacities and back-up systems with high security levels are required. Efficiency and data minimization is an important framework for the design of the processing workflows.

 

In this contribution we as user-turned-developers, want to show how we utilize our toolbox of open-source software (Linux, Bash, R, PostgreSQL/PostGIS, Python, GitLab), for a suitable modularized workflow to meet these challenges.

The first module is tailored to pre-process the data to its specific federal state qualities. Module two and three contain more general functions to grant machine readability. All data is then processed in a data cleaning workflow and imported into our PostgreSQL/PostGIS database.

We use our database for data harmonization by implementing modularized functions to handle different use cases.

The resulting harmonized datasets are provided to research teams with data protection clearance for federal state and year respectively. Harmonized tables are versioned as releases, to either grant reproducibility as well as to provide necessary updates.

Figure 1 Modularized workflow for IACS data processing towards a nation-wide harmonized timeseries

Reproducibly is granted by using script-based procedures that are stored and versioned in GitLab as well as extensive code documentation and automized file-based processing documentation.

Our modularization process lays the foundation for sustainable handling of complex administrative agricultural data and is a first step towards a software development approach.

Literature

European Commission (2025): Integrated Administration and Control System (IACS). Online available  https://agriculture.ec.europa.eu/common-agricultural-policy/financing-cap/assurance-and-audit/managing-payments_en

Deutscher Bundestag (2014): Gesetz über die Verarbeitung von Daten im Rahmen des Integrierten Verwaltungs- und Kontrollsystems nach den unionsrechtlichen Vorschriften für Agrarzahlungen. InVeKoS- Daten-Gesetz - InVeKoSDG, vom 5 (2019). Online available: https://www.gesetze-im-internet.de/invekosdg_2015/

Heidi Leonhardt, Maximilian Wesemeyer, Andreas Eder, Silke Hüttel, Tobia Lakes, Henning Schaak, Stefan Seifert, Saskia Wolff (2024): Use cases and scientific potential of land use data from the EU’s Integrated Administration and Control System: A systematic mapping review, Ecological Indicators, Volume 167, ISSN 1470-160X, https://doi.org/10.1016/j.ecolind.2024.112709.

How to cite: Degen, A., Pao, Y.-C., and Ackermann, A.: A modularized workflow for processing heterogeneous agricultural land use data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17128, https://doi.org/10.5194/egusphere-egu26-17128, 2026.

EGU26-17569 | Orals | ESSI3.4

Latest Developments in Probtest: Probabilistic Testing for Robust CPU/GPU Validation of Scientific Models 

Annika Lauber, Chiara Ghielmini, Daniel Hupp, and Claire Merker

Porting large numerical models to heterogeneous computing architectures introduces significant challenges for software validation and testing, as results from CPU- and GPU-based executions are typically not bit-identical. These differences arise from variations in floating-point arithmetic, execution order, and the use of architecture-specific mathematical libraries. Traditional regression testing approaches based on exact reproducibility therefore become inadequate, particularly in continuous integration (CI) workflows.

Probtest is a lightweight testing framework developed to address this problem in the ICON numerical weather and climate model. It implements a probabilistic, tolerance-based testing strategy that enables robust numerical consistency checks between CPU and GPU runs while remaining fast and resource-efficient. Tolerances are derived from ensembles generated by perturbing prognostic variables in the initial conditions. From a larger ensemble of CPU reference runs, a representative subset is selected to compute variable-specific tolerance ranges that define acceptable numerical deviations. This approach allows reliable validation across architectures without constraining model development or optimization.

Recent developments focus on improving extensibility, usability, and reproducibility. Support for Feedback Output Files (FOF) has been added, enabling consistency checks for observation-based diagnostics in addition to model state variables. Furthermore, Probtest has been fully containerized, with each release published on Docker Hub. This removes local installation barriers, ensures reproducible testing environments, and simplifies integration into CI pipelines and collaborative development workflows. These developments strengthen Probtest as a practical and portable tool for validating ICON across heterogeneous computing platforms.

How to cite: Lauber, A., Ghielmini, C., Hupp, D., and Merker, C.: Latest Developments in Probtest: Probabilistic Testing for Robust CPU/GPU Validation of Scientific Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17569, https://doi.org/10.5194/egusphere-egu26-17569, 2026.

EGU26-17829 | Posters on site | ESSI3.4

Evolution of the EPOS Platform Open Source 

Marco Salvi, Valerio Vinciarelli, Rossana Paciello, Daniele Bailo, Alessandro Crocetta, Kety Giuliacci, Manuela Sbarra, Alessandro Turco, Mario Malitesta, Jean-Baptiste Roquencourt, Martin Carrere, Jan Michalek, Baptiste Roy, and Christopher Card

The development of sustainable and reusable scientific software infrastructures remains a significant challenge in geosciences, particularly when transitioning from single-purpose systems to platforms intended for broader community adoption. This presentation shares experiences and lessons learned from developing the EPOS Platform as an open-source, reusable data integration and visualization system, demonstrating how intentional architectural decisions and tooling investments can transform research infrastructure software into widely adoptable solutions.

The EPOS Platform (European Plate Observing System) initially served as the technical backbone for EPOS ERIC (https://www.epos-eu.org/epos-eric), providing integrated access to solid Earth science data across ten thematic domains. Built on a choreography architecture using Docker and Kubernetes, the system successfully fulfilled its original mandate. However, as other research infrastructures expressed interest in similar capabilities, we recognized the potential for broader impact and initiated a strategic shift toward creating a genuinely reusable open-source platform.

The transition required addressing fundamental challenges in software reusability. Initially, deployment necessitated manual configuration and deep infrastructure knowledge, creating significant adoption barriers. To overcome this, we developed the epos-opensource CLI tool (https://github.com/EPOS-ERIC/epos-opensource), a command-line interface with an integrated terminal user interface (TUI) that reduces deployment from a complex manual process to a single command. This tool enables researchers and developers to deploy fully functional instances locally using either Docker Compose or Kubernetes, significantly accelerating both external adoption and internal development workflows.

We released the complete platform under GPL v3 license, ensuring that all code, including that powering the production EPOS Platform (https://www.ics-c.epos-eu.org/), remains open and community-accessible. Within EPOS ERIC, the open-source release and deployment tooling facilitate rapid provisioning of testing environments for developers and metadata contributors. Comprehensive documentation was developed using Docusaurus, following standard open-source practices to provide installation guides, system architecture references, and user tutorials. The EPOS Platform Open Source has been leveraged to enhance data sharing by multiple research initiatives, including ENVRI-Hub NEXT (https://envri.eu/envri-hub-next/), DT-GEO (https://dtgeo.eu/), IPSES (https://www.ipses-ri.it), and Geo-INQUIRE (https://www.geo-inquire.eu/), demonstrating the platform's versatility across different research contexts.

Our experience demonstrates that developing reusable scientific software requires deliberate investment beyond initial functionality. Key factors include comprehensive documentation following community standards, simplified deployment through user-friendly tooling, architectural flexibility for diverse use cases, and genuine open-source practices where production and community code remain unified. These principles, while resource-intensive, are essential for scientific software to achieve meaningful impact and contribute to a more sustainable, collaborative research infrastructure ecosystem.

This presentation will explore the evolution of the EPOS Platform Open Source, demonstrating how strategic investments in deployment tooling, comprehensive documentation, and architectural flexibility enabled the transformation from a single-purpose infrastructure to a widely adoptable community resource.

How to cite: Salvi, M., Vinciarelli, V., Paciello, R., Bailo, D., Crocetta, A., Giuliacci, K., Sbarra, M., Turco, A., Malitesta, M., Roquencourt, J.-B., Carrere, M., Michalek, J., Roy, B., and Card, C.: Evolution of the EPOS Platform Open Source, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17829, https://doi.org/10.5194/egusphere-egu26-17829, 2026.

EGU26-20382 | Posters on site | ESSI3.4

User-turned-developer: Scientific software development for a national nutrient policy impact monitoring in Germany 

Max Eysholdt, Maximilian Zinnbauer, and Elke Brandes

Many countries in the EU fail to protect their waters adequately from nitrogen and phosphorus inputs (European Environment Agency. 2024), often originating from agricultural sources (Sutton 2011). Germany was found guilty by the European Court of Justice for insufficient implementation of the EU Nitrates Directive, for protection of waters from nutrient pollution from agriculture (European Court of Justice 2018). In response, Germany introduced a monitoring system for assessing the impact of the recently updated application ordinance, which implements the EU Nitrates Directive. This monitoring creates time series of pollution-related spatial indicators ranging from land use to modelled nutrient budgets. Input data on land use sources the Integrated Administration and Control System. The results are used by German authorities for reporting to the EU as well as national and regional water protection policy.

We present the technical concept, infrastructure and workflows established for this data-intensive, long-term project and discuss challenges and limitations when operating in the science-policy nexus. We aim to share good practices in modularization, automation, and reproducibility, and discuss strategies for efficient maintenance of scientific software development in context of long-term, policy-relevant monitoring projects.

Our system is designed to handle heterogeneous data with different levels of data protection requirements related to General Data Protection Regulation (GDPR). A modular structure was chosen to enhance usability and maintenance. Reproducibility is ensured through version-controlled, script-based software development. For efficiency, consistency and the streamlining of workflows reporting is automated and an ever-growing set of user-faced functions is bundled into a package. To ensure the possibility of advances in data preparation and modelling, a submission-based approach was chosen, recalculating all indicator times series each reporting year. This requires robust data management, reproducibility, and resilient workflows to accommodate evolving input data.

We still face challenges in handling Open Science principles, political stakeholder interests as well as GDPR. Similarly, scientific advances lead to updated results which may conflict with the need for clear and unambiguous outcomes of the authorities. Regular deadlines and stakeholder needs resulted in an organically grown code base, and sometimes cause neglection of quality checks and unit testing. Additionally, interaction between reproducible, script-based solutions and “traditional” workflows based on Microsoft Word are inefficient. The changing structure of the yearly gathered data hinders automatization of data processing. Due to this and the annual advances in the processing of the input data, maintaining the database is also challenging.  This we would like to share and discuss with other teams facing similar problem

Our system is tailored to handle heterogeneous and sensitive data of different sources producing reliable results and accommodating advances in data preparation and modelling in the long run. However, navigating technical limitations, good scientific practice and policymakers’ interests is challenging for us.

Literature

European Court of Justice (2018). European Commission against Federal Republic of Germany. Infringement Proceedings ‐ Directive 91/676/EEC.

European Environment Agency. (2024). Europe's state of water 2024: the need for improved water resilience. Publications Office.

Sutton, Mark A. (Ed.) (2011). The European nitrogen assessment. Sources, effects and policy perspectives. Cambridge 2011.

 

How to cite: Eysholdt, M., Zinnbauer, M., and Brandes, E.: User-turned-developer: Scientific software development for a national nutrient policy impact monitoring in Germany, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20382, https://doi.org/10.5194/egusphere-egu26-20382, 2026.

EGU26-21175 | Orals | ESSI3.4

A Python Dynamical Core for Numerical Weather Prediction 

Daniel Hupp, Mauro Bianco, Anurag Dipankar, Till Ehrengruber, Nicoletta Farabullini, Abishek Gopal, Enrique Gonzalez Paredes, Samuel Kellerhals, Xavier Lapillonne, Magdalena Luz, Christoph Müller, Carlos Osuna, Christina Schnadt, William Sawyer, Hannes Vogt, and Yilu Chen

MeteoSwiss uses the ICON model to produce high-resolution weather forecasts at kilometre scale, with GPU support enabled through an OpenACC-based Fortran implementation. While effective, this approach limits portability, maintainability, and development flexibility. Within the EXCLAIM project, we focus on the dynamical core of the model—responsible for approximately 55% of the total runtime—and explore alternatives based on a domain-specific Python framework. In particular, we reimplemented the computational stencils using GT4Py and integrated them into the existing Fortran codebase, enabling the partial replacement of key components. This hybrid approach aims to improve developer productivity and code adaptability while preserving performance. In this contribution, we present our strategy for developing software for a weather and climate model involving multiple institutions and stakeholders. We present several optimisation techniques and compare the performance of the new implementation with the original OpenACC version. Our results show improved computational efficiency alongside a substantial improvement in the development workflow. Finally, we discuss the practical challenges of integrating Python components into operational numerical weather prediction systems.

How to cite: Hupp, D., Bianco, M., Dipankar, A., Ehrengruber, T., Farabullini, N., Gopal, A., Gonzalez Paredes, E., Kellerhals, S., Lapillonne, X., Luz, M., Müller, C., Osuna, C., Schnadt, C., Sawyer, W., Vogt, H., and Chen, Y.: A Python Dynamical Core for Numerical Weather Prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21175, https://doi.org/10.5194/egusphere-egu26-21175, 2026.

EGU26-21181 | ECS | Posters on site | ESSI3.4

Automating Data Quality Checks for Heterogenous Datasets: A scalable approach for IACS data 

Yi-Chen Pao and Boineelo Moyo

The Integrated Administration and Control System (IACS) is a key instrument of the European Union's (EU) Common Agricultural Policy to monitor agricultural subsidies and support evidence-based policy. IACS provides the most comprehensive EU-wide dataset that combines detailed geospatial data with thematic attributes related to land use, livestock and measures, making it highly valuable for research on agri-environmental policies and agrobiodiversity (Leonhardt, et.al., 2024). In Germany, these data are collected independently by 14 federal states, resulting in substantial heterogeneity across datasets in terms of file format, encoding, data structure and level of completeness. These inconsistencies present major challenges for efficient data management, scientific assessments, reproducibility and the long-term reuse of the data.

This contribution presents an ongoing automated framework designed to standardise and validate raw IACS datasets across our data management pipeline, from data collection and harmonisation to data import and long-term management. Our main goal is to reduce redundancy and manual effort in the data quality check process, while enabling scalable and reproducible data quality assurance. The objective is to therefore develop an optimised, non-redundant data check system that captures structural, semantic and geospatial metadata from heterogenous datasets using a single-pass folder scan. To achieve this objective, we focus on the following approaches:

  • Develop an inventory-based data pipeline / architecture: A lightweight inventory object containing metadata for each file in the delivery folder
  • Automate routine and error – prone data quality scripts: Replace manual checks with modular and reusable automated components from a central inventory system
  • Enable reproducible execution and reporting: Implement a Quarto based framework (an open-source system for reproducible computational documents combining code, results and narrative) that produces human readable visualisations for technical and non-technical users

Our system leverages a diverse set of programming tools including R, Quarto, Bash, Python and SQL, from data delivery or collection to data management in the database. The approach is based on an inventory-first architecture: a lightweight yet expressive data structure generated from a single scan of raw input folder with different types of data formats. The inventory then captures essential metadata of each file such as file types, attribute schemas, geospatial extents, and identifier patterns (e.g., farm identifier, land parcel identifier). A consolidated framework of all data check scripts then enables all subsequent quality-check modules to operate efficiently without repeated file access. Executing the consolidated framework performs a range of automated data quality checks such as file integrity verification, cross-file joinability analysis, schema consistency assessment, and geospatial coherence analysis.

The resulting output in the form of an interactive Quarto dashboard then provides a comprehensive first assessment of the delivered data, where all essential metadata and errors of each file can be derived and inspected in one instance. This workflow not only minimises manual work of checking each file separately and error propagation but also ensures traceable, documented logs.

Our results show how implementing such automated data checks considerably accelerates harmonization processes and improves the data management lifecycle.

How to cite: Pao, Y.-C. and Moyo, B.: Automating Data Quality Checks for Heterogenous Datasets: A scalable approach for IACS data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21181, https://doi.org/10.5194/egusphere-egu26-21181, 2026.

EGU26-21322 | Posters on site | ESSI3.4

SIrocco: a new workflow tool for Climate and Weather including explicit data representation and ICON support 

Matthieu Leclair, Julian Geiger, Alexander Goscinski, and Rico Häuselmann

With the increase in simulation resolution, climate and weather models are now potentially outputting petabytes of data. The largest projects can thus require complex workflows tightly integrating pre-processing, computing, post-processing, monitoring, potential downstream applications or archiving. We introduce here Sirocco, a new climate and weather workflow tool written in Python in collaboration between ETHZ, PSI and CSCS with a special care for the ICON model. 

Sirocco is written with separation of concerns in mind, where users should only care about expressing their desired workflow and bringing the scripts/sources for each task independently. That's why "Sirocco" first designates a user-friendly yaml based configuration format. Inspired by cylc and AiiDA, it describes the workflow graph by equally integrating data nodes (input and output) alongside task nodes. Workflows thus become truly composable, in the sense that no task is making any assumption on the behavior of others.

Sirocco currently defines two types of tasks, called "plugins". The "shell" plugin is dedicated to tasks for which users provide their own main executable, including any auxiliary set of files. The only requirement is the ability to interface with Sirocco, either with executables accepting command line arguments and environment variables and/or by parsing a yaml file providing the necessary context for task execution. The "icon" plugin is a dedicated user friendly interface to the ICON model. On top of the integration to Sirocco workflows, it provides easy ways of handling matters like date changing, namelist modifications, restart files or predefined setups for target machine and architecture. By design, other plugins can be written to facilitate the integration of any other application/model.

Once an internal representation is generated from the configuration file, two possible back-ends can orchestrate the workflow. The first one, called "stand-alone", is entirely implemented inside Sirocco and runs autonomously on the target machine, only relying on the HPC scheduler daemon to keep the workflow running. The second one interfaces with the low-level workflow library AiiDA and its satellite packages, running on a dedicated server with its own daemon and dumping workflow metadata in a queryable database. Both orchestrators implement the novel concept of a deep dynamical task front that propagates through the graph, enabling the ahead-of-time submission of an arbitrary number of task generations.

At the end of the day, Sirocco not only provides the ability to run complex workflows and a nice interface to ICON but also, through its workflow manager nature, facilitates shareability and reproducibility in the community.

How to cite: Leclair, M., Geiger, J., Goscinski, A., and Häuselmann, R.: SIrocco: a new workflow tool for Climate and Weather including explicit data representation and ICON support, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21322, https://doi.org/10.5194/egusphere-egu26-21322, 2026.

EGU26-21348 | Posters on site | ESSI3.4

CAES3AR: Collaborative and Efficient Scientific Software Support Architecture 

Florian Wagner, Camilla Lüttgens, Andrea Balza Morales, Marc S. Boxberg, Marcel Nellesen, and Marius Politze

Scientific software is essential for accelerating research and enabling transparent, reproducible results, but increasing adoption also increases support demands that can overwhelm small academic development teams. Since most scientists are not trained as software engineers, early-stage research software often lacks the resources and structure needed for broader use, making streamlined support workflows crucial for both users and developers. Addressing these issues is essential to ensure that researchers can focus on their core activities while streamlining processes that benefit both users and developers.

Our project CAES3AR (Collaborative and Efficient Scientific Software Support Architecture) aims to provide researchers with a more open and efficient infrastructure for software support by developing a collaborative architecture. The framework is currently being developed and evaluated using pyGIMLi, an open-source library for modeling and inversion in geophysics (www.pygimli.org), while being designed to remain transferable to a broad range of open-source projects. Thanks to its practicality and gallery of existing examples, pyGIMLi has become widely adopted in the near-surface geophysical community. At the same time, its use across diverse user environments introduces recurring support challenges, since variations in operating systems and installed dependencies can make issue reproduction and debugging time-intensive, which often reduces the capacity for methodological and software innovation.

To address these challenges efficiently, the CAES3AR framework aims to automate key aspects of user support through a generic toolchain that integrates seamlessly with existing infrastructures such as GitHub and Jupyter. It facilitates user engagement by allowing them to create GitHub or GitLab issues that include links to temporary code execution environments (e.g., JupyterLab) equipped with collaborative editing features—potentially integrated with existing JupyterHub and cloud-based infrastructures. Additionally, automated bots powered by GitHub Actions or GitLab jobs will provide real-time feedback on whether issues exist across all platforms and with the latest software versions. If a problem persists, supporters can directly modify the user's code within Jupyter without requiring any downloads or installations. Proposed changes will be presented as formatted code alterations (“diffs”) attributed to their authors in the Git issue for future reference, ensuring clarity and continuity even after the temporary JupyterHub instance is no longer available.

We recently hosted a community workshop to assess developer and user needs, identify challenges in current support practices, and gather requirements for practical adoption. This presentation summarizes key findings from those discussions and introduces early CAES3AR prototypes developed for the pyGIMLi ecosystem. As CAES3AR remains in active development, we conclude by inviting community feedback on additional features and design priorities, with the broader aim of ensuring transferability and long-term utility across multiple open-source scientific software projects.

Project website: https://caesar.pages.rwth-aachen.de/

 

How to cite: Wagner, F., Lüttgens, C., Balza Morales, A., Boxberg, M. S., Nellesen, M., and Politze, M.: CAES3AR: Collaborative and Efficient Scientific Software Support Architecture, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21348, https://doi.org/10.5194/egusphere-egu26-21348, 2026.

EGU26-23282 | Posters on site | ESSI3.4

Evolving Scientific Software in Long-Running Observatories: Lessons from the TERENO Sensor Management Migration 

Ulrich Loup, Werner Küpper, Christof Lorenz, Rainer Gasche, Ralf Kunkel, Ralf Gründling, Jannis Groh, Nils Brinckmann, Jan Bumberger, Marc Hanisch, Tobias Kuhnert, Rubankumar Moorthy, Florian Obersteiner, David Schäfer, and Thomas Schnicke

Abstract:

Scientific software in geosciences often grows organically: initial solutions
are developed within small teams to meet immediate research needs, and over time
they evolve into critical infrastructure. While this organic growth can be
highly effective, it frequently leads to challenges in maintainability,
documentation, and reuse when systems are expected to support larger communities
or integrate with new platforms. In this contribution, we share lessons learned
from evolving the software infrastructure of the TERENO environmental observatories.

For more than a decade, TERENO relied on tightly coupled systems in which
observational data and sensor metadata were managed together. This data
infrastructure proved robust in daily operations but gradually accumulated
inconsistencies, implicit conventions, and project-specific extensions that were
insufficiently documented. As TERENO is now being integrated into the Earth &
Environment DataHub, these limitations became visible and required a systematic
rethinking of how sensor and measurement metadata are managed.

As part of the infrastructure redesign within the Earth & Environment DataHub
initiative, we adopted the Helmholtz Sensor Management System (SMS), an open,
community-driven software platform. To support the transition, we developed and
extended the Python tool ODM2SMS, which enables reproducible and configurable
migration of metadata from the legacy system into SMS. This process exposed
several common pitfalls in scientific software development: hidden assumptions
in data structures, incomplete documentation, and software that worked well for
its original developers but was hard to adapt for new use cases.

We addressed these challenges by applying a set of pragmatic good practices.
These included increasing modularity and configurability in ODM2SMS, explicitly
documenting previously implicit rules, and combining automated migration steps
with manual review where scientific context was required. A particularly
instructive example is the migration of complex lysimeter installations,
involving hundreds of interconnected devices. This case highlighted the
importance of clear abstractions, shared terminology, and close interaction
between users and developers.

Our contribution reflects on how community engagement, open development, and
incremental refactoring can improve long-lived scientific software without
disrupting ongoing research. We conclude by discussing transferable lessons for
researchers facing similar challenges: balancing rapid development with
sustainability, making software usable beyond its original context, and turning
legacy systems into maintainable, future-ready tools.

How to cite: Loup, U., Küpper, W., Lorenz, C., Gasche, R., Kunkel, R., Gründling, R., Groh, J., Brinckmann, N., Bumberger, J., Hanisch, M., Kuhnert, T., Moorthy, R., Obersteiner, F., Schäfer, D., and Schnicke, T.: Evolving Scientific Software in Long-Running Observatories: Lessons from the TERENO Sensor Management Migration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23282, https://doi.org/10.5194/egusphere-egu26-23282, 2026.

EGU26-1739 | ECS | Posters on site | HS3.8

Missing data imputation in epidemiology: a comparison between MICE and Machine Learning methods 

Mahmoud Hashoush, Emmanuelle Cadot, and Franco Alberto Cardillo

Missing data represents a challenge in large-scale epidemiological studies as it can introduce a strong and negative bias in the final estimates when not handled appropriately. This issue is particularly relevant in environment health research due to complex relationships between the exposure to risk factors and delayed outcomes. In this work, we evaluate the effectiveness of statistical and Machine Learning (ML) approaches to fill in missing values in data we collected to assess the potential impact on public health of gold mining activities in the Ecuadorian Amazon.

There is growing concern regarding the adverse effects on human health in the Ecuadorian Amazon caused by the environmental impact of gold mining activities in the area. To investigate potential associations with adverse birth outcomes, we collected data published by the Ecuadorian National Institute of Statistics and Census (INEC) relative to the annual live birth and fetal death cases in the years from 2014 to 2023. As it is typical in large-scale epidemiological studies, the data contain a proportion of missing values, likely related to the registration and the data entry process. 

Addressing missing values is considered important for the correct assignment of cases from one hand and the characterisation of risk factors from another. Furthermore, it enables the modelling process when searching for associations between exposure and outcome without erroneous under- or over-reporting of odds ratios (Type I and Type II errors). Currently, the most common approach in epidemiology is to use statistical methods and, specifically, Multivariate Imputation by Chained Equations (MICE), normally instantiated with parametric conditional models. MICE imputes missing values by repeatedly predicting each incomplete variable from the others using standard regression models. In most applications, these predictions rely on linear or generalised linear relationships between variables. This can reduce its effectiveness in predicting missing values in presence of complex, non-linear interactions about variables. Machine Learning represents an interesting alternative as it capture complex, non-linear relationships beyond the linear models typically assumed in MICE, are more flexible with respect to departures from missing-at-random patterns, and reduce the risk of model misspecification by relying on data-driven, implicit model selection rather than requiring the analyst to pre-specify an imputation model.

In this study, we present a robust experimental comparison between MICE and several ML-based imputation approaches applied to the Ecuadorian birth data. We assess their performance and discuss the respective strengths and limitations within an epidemiological context.

How to cite: Hashoush, M., Cadot, E., and Alberto Cardillo, F.: Missing data imputation in epidemiology: a comparison between MICE and Machine Learning methods, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1739, https://doi.org/10.5194/egusphere-egu26-1739, 2026.

The lack of extensive and functional ground observation networks introduces satellite-based rainfall products as an alternative. However, these datasets require prior evaluation. This study investigates the performance of four satellite- and gauge-based rainfall products: the Climate Hazards Group Infrared Precipitation with Station data version v2.0 (CHIRPS); Precipitation Estimation from Remotely Sensed Information using Artificial Neural Networks Climate Data Record (PERSIANN); Tropical Applications of Meteorology using Satellite data and ground-based observations (TAMSAT); and the Global Precipitation Climatology Centre full daily data (GPCC).

The assessment was conducted using grid-to-point comparisons at different time scales, and hydrological modelling over the Mono River Basin, located in the Republics of Benin and Togo. To assess the suitability of the four products for flood purposes, a two-step approach was applied: (1) a satellite-only approach in which each product was used as input to the HBV-light hydrological model for runoff simulation, and (2) an observation-satellite approach in which gaps in observation data were filled using each product prior to the hydrological modelling. In all simulations, areal precipitation was derived with kriging before being input into HBV-light. On the one hand, the simulation with CHIRPS-only showed poor performance (NSE = -0.08 during calibration and -0.22 during validation), while the simulations with PERSIANN-only, TAMSAT-only, and GPCC-only yielded moderate performance, with NSE values ranging from 0.5 to 0.67. On the other hand, simulations with the observation-satellite combinations also showed moderate performances, with NSE values between 0.55 and 0.69, including for the observation-CHIRPS case.

The poor performance of the CHIRPS-only simulation, combined with the similar performance of all observation-satellite combinations, indicates that the quality of the satellite product used for gap filling plays a limited role. Moreover, the absence of significant improvement when using observation-satellite combinations compared to their satellite-only counterparts (except for CHIRPS) suggests that gap filling with satellite products does not necessarily enhance data quality. These results indicate that, in the Mono River Basin, gap filling may not be necessary when spatial interpolation methods such as kriging are applied.

How to cite: Houngue, N.: When More Data Is Not Better: Evaluating Satellite Rainfall Products in a Data-Scarce River Basin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3102, https://doi.org/10.5194/egusphere-egu26-3102, 2026.

EGU26-3221 | Orals | HS3.8

Disentangling Sources of Uncertainty in Hydrologic Projections Using Multiple Climate Forcings, Bias-Correction Techniques, and Shared Socioeconomic Pathways 

Rocky Talchabhadel, Sunil Bista, Saurav Bhattarai, Subash Poudel, Amisha Bhandari, Sandhya Khanal, Aashish Gautam, Yogesh Bhattarai, Sanjib Sharma, and Nawa Raj Pradhan

Meteorological forcings under different climate scenarios exert substantial control over hydrologic-hydrological processes in watersheds and river systems. This study presents a comprehensive assessment of uncertainty in hydrologic projections by integrating a wide range of climate forcings, multiple bias-correction approaches, and several Shared Socioeconomic Pathways (SSPs). Specifically, we (i) quantify the total uncertainty in projected hydrologic responses, (ii) attribute uncertainty to individual sources, and (iii) examine how uncertainty propagates along the hydroclimatic modeling chain. The analysis is demonstrated for a range of watersheds using a fully calibrated Soil and Water Assessment Tool (SWAT) model. The hydrologic simulations are forced by outputs from thirty global climate models (GCMs) participating in the Coupled Model Intercomparison Project Phase 6 (CMIP6), obtained from the NASA Earth Exchange Global Daily Downscaled Projections (NEX-GDDP-CMIP6) dataset at a spatial resolution of 0.25° (~25 km) under two SSPs. To further refine the climate inputs, a linear bias-correction method is applied to daily temperature and precipitation time series to align long-term mean monthly values during the reference period (1985–2014) with PRISM observations. A total of four bias-correction scenarios are considered: (1) original NEX-GDDP-CMIP6 data, (2) precipitation-corrected data, (3) temperature-corrected data, and (4) jointly corrected temperature and precipitation data. This framework yields four forcing scenarios for each GCM–SSP combination, resulting in a total of 240 simulations (4 × 30 GCMs × 2 SSPs) for each watershed. Streamflow changes are evaluated for the near-future period (2031-2060) and far future period (2061-2090), relative to the historical baseline (1985-2014). Changes in probability distributions and cumulative distribution functions are analyzed across climate models, bias-correction methods, and SSPs. In addition, the relative contributions of individual uncertainty sources are quantified at monthly, seasonal, and annual time scales. By systematically accounting for uncertainties arising from climate forcings, bias-correction techniques, and socioeconomic pathways, this study provides a robust characterization of the range of plausible hydrologic futures. Such uncertainty-informed streamflow projections are essential for water-resources planning, flood and drought risk management, and the development of effective long-term water-management strategies.

How to cite: Talchabhadel, R., Bista, S., Bhattarai, S., Poudel, S., Bhandari, A., Khanal, S., Gautam, A., Bhattarai, Y., Sharma, S., and Pradhan, N. R.: Disentangling Sources of Uncertainty in Hydrologic Projections Using Multiple Climate Forcings, Bias-Correction Techniques, and Shared Socioeconomic Pathways, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3221, https://doi.org/10.5194/egusphere-egu26-3221, 2026.

EGU26-6637 | Posters on site | HS3.8

GeoAI-based augmentation of multi-source urban GIS 

Salem Benferhat, Nanée Chahinian, Carole Delenne, Ines Couso Blanco, Luciano Sanchez Ramos, and Zoltan Kato
This presentation addresses a major challenge: fully leveraging the potential of geospatial data to improve Geographic Information Systems (GIS). Using urban flooding as a case study, it aims to integrate heterogeneous data sources of varying nature and quality levels in order to enhance both the expressiveness and reliability of GIS.
 
This work presents ongoing and planned research activities within the ATLAS CHIST-ERA project, which is entirely dedicated to this objective through a multidisciplinary approach. The project mobilizes complementary expertise in GIS, artificial intelligence, machine learning, computer vision and 2D/3D image analysis and object detection, statistics, urban network mapping, as well as geoalignment techniques.
 
The presentation is structured around two main objectives, both oriented toward GIS enrichment, with direct applications for flood risk management.
 
The first objective consists of combining and integrating external data within GIS. This approach enables seamless data integration and facilitates the revision, completion, and enrichment of existing datasets, while improving their expressiveness, particularly through the introduction of 3D representations. Such enriched representations are essential for accurately modeling surface runoff, flow paths, and hydraulic connectivity in urban environments subject to flooding.
 
The second objective focuses on integrating imperfect or uncertain data, such as amateur videos, crowdsourced observations, or data lacking precise georeferencing. To address these limitations, the project relies notably on the use of variational autoencoders for processing imprecise data, and proposes uncertainty and imprecision management mechanisms aimed at improving data quality by reducing inaccuracies and explicitly modeling confidence levels.
 
Acknowledgments :
This work was supported by the CHIST-ERA project ATLAS "GeoAI-based augmentation of multi-source urban GIS" under grant numbers CHIST-ERA-23-MultiGIS-02 and ANR-24-CHR4-0005 (French National Research Agency).

How to cite: Benferhat, S., Chahinian, N., Delenne, C., Couso Blanco, I., Sanchez Ramos, L., and Kato, Z.: GeoAI-based augmentation of multi-source urban GIS, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6637, https://doi.org/10.5194/egusphere-egu26-6637, 2026.

EGU26-6933 | ECS | Orals | HS3.8

Integration and Alignment of Multiple Water Network Data Sources 

Omar Et-targuy, Carole Delenne, Salem Benferhat, and Ahlame Begdouri

Wastewater network management relies on geographic data from multiple sources, which creates significant integration challenges: spatial inconsistencies, incomplete coverage, and varying levels of precision.

Although different data sources may cover the same portion of the network, they are generally produced in different contexts or at different times. This can result in discrepancies in the descriptions of the physical infrastructure of the wastewater network: some elements may be accurately represented in one source but absent in another, while other objects may be described slightly differently across sources. Furthermore, for certain parts of the network, the structure itself may vary depending on the source. Consequently, any operation to merge datasets or build a global network representation requires matching the objects described by each source in order to identify those corresponding to the same physical element, to recognize objects present in multiple sources, and to distinguish those with no correspondence in other datasets.

In this work, we propose a data integration methodology to address disparities among these data sources and to match the various elements of wastewater networks. This approach establishes correspondences between multiple datasets representing the same infrastructure from different sources. By combining spatial and structural information, the method identifies matching components across datasets and produces a unified representation that leverages the complementary information from each source while resolving conflicts and inconsistencies.

The approach has been validated on real-world wastewater network data from multiple sources and covering different time periods. The results demonstrate high integration accuracy. This methodology enables a complete and consistent representation of wastewater networks, addressing the challenges of data heterogeneity inherent in multi-source infrastructure management.

How to cite: Et-targuy, O., Delenne, C., Benferhat, S., and Begdouri, A.: Integration and Alignment of Multiple Water Network Data Sources, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6933, https://doi.org/10.5194/egusphere-egu26-6933, 2026.

EGU26-7251 | Orals | HS3.8

 Cross-analysis of Multisource Data for Geolocation of Non-georeferenced Urban Infrastructure Data 

Thanh Ma, Salem Benferhat, Minh Thu Tran Nguyen, Nanée Chahinian, Carole Delenne, and Thanh-Nghi Do

Geographic Information Systems (GIS) are reference tools for representing, storing, analyzing, and visualizing geolocated data, particularly those related to urban infrastructures such as water networks. In addition to GIS reference data, there exists a significant amount of complementary data, referred to here as external data, generally produced in specific contexts such as urban network maintenance. When properly exploited, these external data sources, which are rich in information, can enhance GIS and help address the issue of missing data. However, these external data are often not geolocated, which makes their integration into GIS particularly complex.

The main objective of this work is to propose artificial intelligence–based methodologies to geolocate non-georeferenced external data, particularly maps related to urban water networks, by leveraging multisource data cross-analysis. The proposed approach relies on the joint exploitation of geolocated GIS data and external data lacking geolocation. It consists in analyzing maps using object detection techniques to extract characteristic elements, such as buildings or specific structures, which are then matched with corresponding entities available in the relevant GIS. By exploring different geographic areas of the same spatial extent as the maps and assessing the degree of similarity between the extracted elements and those referenced in the GIS, the method enables the identification of the most plausible area of correspondence and, ultimately, the geolocation of the maps in question.

This work addresses several major challenges in the context of geolocating external data using GIS data. The first challenge concerns the identification and selection of relevant elements capable of effectively guiding the search within available GIS. The second challenge lies in accounting for the sometimes limited reliability of object detection systems during the matching process. The third challenge involves defining appropriate similarity measures and selecting sufficiently discriminative elements for the matching process. Finally, the fourth challenge is algorithmic in nature, given that a map generally represents only a limited portion of a GIS, which raises issues similar to those encountered in large-scale matching approaches.

Acknowledgments :
This work was supported by the CHIST-ERA project ATLAS "GeoAI-based augmentation of multi-source urban GIS" under grant numbers CHIST-ERA-23-MultiGIS-02 and ANR-24-CHR4-0005 (French National Research Agency).

How to cite: Ma, T., Benferhat, S., Tran Nguyen, M. T., Chahinian, N., Delenne, C., and Do, T.-N.:  Cross-analysis of Multisource Data for Geolocation of Non-georeferenced Urban Infrastructure Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7251, https://doi.org/10.5194/egusphere-egu26-7251, 2026.

EGU26-7685 | ECS | Posters on site | HS3.8

Data assimilation to retrieve unknown bathymetry in shallow water model 

Flavien Baudu, Carole Delenne, Thibault Catry, Sophie Ricci, Ludovic Cassan, Vincent Herbreteau, and Renaud Hostache

Floods are among the most destructive and costly natural disasters. While risk assessment and management have helped mitigate their impact in recent decades, climate change is expected to increase both their frequency and severity. This underscores the urgent need for predictive tools to better anticipate and prevent the adverse effects of flooding. Two-dimensional Shallow-Water (SW) hydraulic models offer a reliable solution for flood prediction, providing critical information such as floodplain extent, water levels and flow velocities. However, these models require boundary conditions (such as input flows), precise topography and bathymetry (i.e. riverbed geometry) as well as parameters to be calibrated (such as terrain roughness.  Unfortunately, such data are often sparse or entirely unavailable in many regions due to the high cost and logistical challenges of in situ measurements. In particular, if the topography can be obtained using LiDAR acquisition of Numerical Terrain Models, the bathymetry remains unaccessible because LiDAR signal does not pass through the water surface.

In this context, Data Assimilation (DA)—a method that optimally combines uncertain models with observations—becomes particularly valuable for estimating such missing data or parameters. Our study proposes an innovative approach to reconstruct riverbed geometry by assimilating flood extent information derived from satellite imagery, specifically Synthetic Aperture Radar (SAR) data, which can reliably detect floodwater extents.

To account for observational uncertainty, we generate a probabilistic flood map from SAR images, where each pixel’s value represents its probability of being water, based on observed backscatter. Using a tempered particle filter (TPF), we assimilate multiple SAR-derived probabilistic flood maps into an ensemble of hydraulic simulations (referred to as "particles"). These simulations share the same model architecture but incorporate randomly sampled riverbed geometries. 

To evaluate our methodology, we conducted a synthetic twin experiment based on a real-world case study of the River Severn near Tewkesbury, UK—a region prone to frequent flooding. We first perform a hydraulic simulation (the "control run") using a reference riverbed geometry and realistic boundary conditions. From this simulation, we generate several synthetic probabilistic flood maps, which were then assimilated into a second simulation to estimate the riverbed geometry using the TPF.

Our results demonstrate the effectiveness of this approach: the estimated riverbed geometry closely matches the reference. Additionally, contingency maps reveal strong agreement between the flood extents predicted by the control run and those obtained through the DA experiment.

How to cite: Baudu, F., Delenne, C., Catry, T., Ricci, S., Cassan, L., Herbreteau, V., and Hostache, R.: Data assimilation to retrieve unknown bathymetry in shallow water model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7685, https://doi.org/10.5194/egusphere-egu26-7685, 2026.

EGU26-7760 | Posters on site | HS3.8

Anomaly detection in wastewater pipeline videos using self-attention 

Carole Delenne, Ti-Hon Nguyen, Minh-Thu Tran-Nguyen, and Salem Benferhat

Data related to urban infrastructures often come from multiple sources and exist in a wide variety of formats, such as Geographic Information Systems (GIS), textual information, numerical databases, images, or videos, which can make their processing, querying, and analysis complex. This work falls within this context and aims to propose new approaches for the management of heterogeneous data in stormwater and wastewater networks.

More specifically, we focus on video data, particularly Closed-Circuit Television (CCTV) inspection videos of sewer pipelines. These videos are essential for the management and maintenance of urban networks. On the one hand, they enable the identification of anomalies that may affect the integrity of pipelines, such as blockages or structural degradation. On the other hand, they provide key information on the structural properties of pipelines and networks, including pipe diameter and the direction of wastewater flow.

We propose a classification algorithm for wastewater inspection videos aimed at detecting major anomalies in CCTV inspection sequences of sewer networks, with a particular emphasis on identifying variations in pipe diameter, internal cracks, chemical corrosion, and the presence of turbid water within the pipelines. This task is crucial for predictive maintenance and hydraulic modeling of sewer systems. Information related to the identification of variations in pipe diameter can also be leveraged to enrich and complete missing pipe diameter attributes in Geographic Information Systems.

Our approach is based on the Video Vision Transformer (ViViT) and TimeSformer architectures, which effectively capture both spatial and temporal relationships in video data. We also describe various methodologies for generating training datasets from a subset of manually annotated images. Experimental results obtained on real-world CCTV sewer inspection videos provided by Montpellier Méditerranée Métropole demonstrate promising performance in anomaly detection.

How to cite: Delenne, C., Nguyen, T.-H., Tran-Nguyen, M.-T., and Benferhat, S.: Anomaly detection in wastewater pipeline videos using self-attention, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7760, https://doi.org/10.5194/egusphere-egu26-7760, 2026.

EGU26-7776 | ECS | Posters on site | HS3.8

CawSAR: an open-source framework for preprocessing hydroclimatic data in physically based hydrological modelling 

Tristan Bourgeois, Nicolas Flipo, Marie Pettenati, and Hervé Noel

Water resource management is a major challenge for the coming decades. Its effective application across diverse territories therefore relies on an accurate representation of hydrological processes, generally achieved through physically based distributed hydrological models which in turn depend on spatially consistent and representative hydroclimatic forcing. At regional scales, capturing local variability in hydroclimatic drivers (precipitation, temperature, evapotranspiration) often requires combining datasets with different spatial resolutions and methodological assumptions.

Within the Eau-SPRA project (ADEME, France 2030 Programme), the CaWaQS model (Flipo et al., 2022; Flipo et al., 2023) is applied to the Loire River basin to support socio-hydrological modelling from regional to local scales. CaWaQS is a coupled distributed surface–subsurface hydrological model simulating both river discharge and groundwater dynamics. It currently lacks an explicit snow representation, which can significantly affect hydrological dynamics across scales, particularly in large river basins such as the Loire and under climate change conditions (Valéry et al., 2014).

To address these challenges, we developed CawSAR (CaWaQS Snow Accounting Routine), an open-source Python-based preprocessing framework designed to harmonize multi-source climate data (e.g. reanalysis products, radar observations) over a target study area. Based on a 3D matrix representation (time, x, y) of climate fields, it integrates multiple functionalities within a single, reproducible workflow. Climate data are harmonized through systematic downscaling, upscaling and regridding performed on a grid-cell basis using physical external-drift adjustments (altimetric gradient). CawSAR also enables cross-comparison of climate data sources across different spatio-temporal scales and implements a degree-day snow model to compute snow accumulation and melt. Finally, it generates liquid input time series (sum of liquid rainfall and snowmelt) fully compatible with the CaWaQS core model, ensuring direct integration into hydrological simulations.

Applied to the Loire basin, CawSAR illustrates how physically based preprocessing and multi-source harmonization enhance hydroclimatic forcing consistency for regional-scale hydrological modelling.

How to cite: Bourgeois, T., Flipo, N., Pettenati, M., and Noel, H.: CawSAR: an open-source framework for preprocessing hydroclimatic data in physically based hydrological modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7776, https://doi.org/10.5194/egusphere-egu26-7776, 2026.

EGU26-9507 | ECS | Posters on site | HS3.8

From Imperfect Sewer Data to Coherent Topology: A Graph-Based Approach  

Batoul Haydar, Nanée Chahinian, and Claude Pasquier

Urban sewer networks are critical infrastructures that support residents' everyday life and ensure the collection and transportation of wastewater and stormwater. Yet operational datasets describing these networks are frequently imperfect: pipes may be missing, connectivity may be fragmented, and flow direction may be inconsistent due to incomplete attributes (e.g., invert levels, slope) or digitizing errors. We present a topology-focused study that transforms sewer data into a directed network by combining (i) graph-based representation and (ii) geometry-based consistency checks and rules. Starting from a directed (multi)graph built from available pipe and node geometries, which represent the edges and nodes in the graph, we detect topological anomalies including disconnected components, missing connections, dead ends, and closed loops.

When two pipes converge at a manhole with no outgoing pipe, it forms a non-outlet sink. To resolve this, we apply a two-stage methodology: edge orientation to reduce flow inconsistencies and resolve any sink nodes, followed by targeted edge addition to reconnect remaining disconnected components when reversals alone are insufficient. We test feasibility of the approach on a large open-access urban sewer dataset. The results illustrate how topology-oriented methods can still be applied to establish a well-connected network when data attributes are missing or unreliable.

How to cite: Haydar, B., Chahinian, N., and Pasquier, C.: From Imperfect Sewer Data to Coherent Topology: A Graph-Based Approach , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9507, https://doi.org/10.5194/egusphere-egu26-9507, 2026.

EGU26-11107 | Orals | HS3.8

The effects of droughts on pumping fields at the watershed scale: building a model from a heterogeneous dataset. 

Jordan Labbe, Hélène Celle, Julie Albaric, Pierre Nevers, Gilles Mailhot, Jean-Luc Devidal, and Nathalie Nicolau

Water management is becoming an increasingly complex task that must account for not only climate change but socio-economic pressures as well. This is particularly true in the case of alluvial aquifers which are often connected to surface waters, thus requiring a watershed scale policy. Conflicts of use might emerge especially during droughts which are occurring more frequently. In this context, the alluvial aquifer of the Allier River (France) is an interesting case study. This is a major regional resource for drinking water, industries and irrigation which extends over 210 km long between Langeac and the confluence with the Loire River. The Naussac dam keeps the Allier River at a minimum flow rate and secures water uses downstream, but the summer drought of 2023 was extreme and the dam was almost completely emptied. If this situation were to repeat itself over a longer period, the consequences on the productivity of pumping fields implanted on the alluvial aquifer are unknown. This work is part of the MODALL² project in which we propose to build a transient model of the alluvial aquifer using MODFLOW (Groundwater Vistas 8). One of the main challenges is to gather and organize a set of often heterogeneous data (incomplete time series, spatial data sparsely distributed etc.) from various sources. With the intention of improving the existing network, 50 additional water loggers have been deployed for groundwater level monitoring. 30 Electrical Resistivity Tomography (ERT) profiles were carried out to refine the thickness of alluvial deposits on the well-fields and thus, the geometry of the model. Given the elongated dimension of the alluvial aquifer, the study area is divided into 9 sub-models with which a ‘cascade modelling’ is performed. The purpose is to better understand how droughts spread across the whole hydrosystem and to what extent the pumping fields will be affected. ERT surveys have revealed that the thickness of alluvial deposits varies significantly from one site to another, ranging from 5 to 15 m downstream where the alluvial plain is more widespread. Hydrodynamic data show the influence of the river on groundwater level variations depending on the distance from the river. Lastly, the heterogeneity of the input datasets introduces uncertainty into the model that will need to be estimated. Beyond the potential to use modeling to anticipate future water crises, this work also proposes a methodology for handling large-scale heterogeneous datasets.

How to cite: Labbe, J., Celle, H., Albaric, J., Nevers, P., Mailhot, G., Devidal, J.-L., and Nicolau, N.: The effects of droughts on pumping fields at the watershed scale: building a model from a heterogeneous dataset., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11107, https://doi.org/10.5194/egusphere-egu26-11107, 2026.

EGU26-11579 | ECS | Orals | HS3.8

A comparative benchmark of tabular, sequential, and graph-based models for well-log imputation 

Wendinkonté Fabrice Cédric Sawadogo, Romain Chassagne, and Olivier Atteia

Well-log datasets commonly contain missing values due to acquisition issues, operational constraints, and economic limitations, which complicate quantitative subsurface analysis and useful extraction of information in geothermal and more largely subsurface characterisation. Imputation is therefore a key preprocessing step, yet many existing approaches primarily focus on within-well continuity and treat the problem as a depth-wise or time-series task, often overlooking spatial redundancy between neighbouring wells.

In this contribution, we compare three complementary modeling paradigms for well-log imputation: tabular machine-learning methods, sequential deep-learning models, and spatially informed graph-based approaches. The comparison is conducted within a unified and reproducible experimental framework based on cross-well validation and realistic missingness scenarios, including isolated gaps as well as extended block-wise and complete log-wise gaps.

Results highlight clear differences in behaviour across modeling families. Tabular methods exhibit limited robustness when missing values become structured, while sequential models improve depth-wise continuity but remain sensitive to large gaps and absent logs. In contrast, spatially informed graph-based models show increased stability by exploiting inter-well relationships, leading to more coherent reconstructions at the field scale.

These results suggest that evaluating imputation quality solely through local error metrics is insufficient for realistic subsurface applications. By emphasizing the importance of spatial coherence and inter-well information, this study supports the use of spatially aware formulations as a valuable alternative to purely depth-wise approaches for geothermal and broader subsurface characterization workflows.

How to cite: Sawadogo, W. F. C., Chassagne, R., and Atteia, O.: A comparative benchmark of tabular, sequential, and graph-based models for well-log imputation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11579, https://doi.org/10.5194/egusphere-egu26-11579, 2026.

EGU26-11636 | ECS | Orals | HS3.8

Unsupervised pattern recognition for imperfect datasets: a visual workflow for plausibility checks and regime diagnosis in high-dimensional environmental time series 

Kenneth Gutiérrez, Gunnar Lischeid, Gökben Demir, Maren Dubbert, Alexander Knohl, and Christian Markwitz

Data imperfection is characterized by fragmentation, sensor failures, and high-dimensional noise. This remains a persistent challenge in environmental monitoring. As observation networks expand to capture heterogeneous soil-atmosphere interactions, traditional quality control methods based on rigid statistical thresholds often struggle to distinguish between sensor errors and genuine, non-linear system dynamics. This study presents a methodological development for knowledge extraction from imperfect and fragmented data, employing a multivariate visualization workflow that combines Principal Component Analysis (PCA) and Self-Organizing Maps (SOM) with Sammon Mapping.

We applied this unsupervised learning approach to a high-dimensional dataset (~100 variables) from a field-scale agricultural system, including measurements of soil moisture and temperature, eddy covariance-derived CO2, energy fluxes, radiation, wind, precipitation, groundwater level and discharge.

This allowed us to compare a discontinuous period in 2024 against a continuous period in 2025. The results demonstrate the method's robustness in extracting coherent structural patterns despite data incompleteness. While PCA effectively isolated the dominant thermodynamic baselines from high-frequency hydrologic events, the topological SOM projection provided a rapid, visual plausibility check.

The visualization facilitated the identification of possible irregularities in the sensors as spatial outliers in the 2024 dataset, facilitating instant anomaly detection without manual time-series inspection. Furthermore, the method successfully captured shifts in system dynamics, such as the decoupling of surface moisture from groundwater, validating its utility for identifying physical regimes in heterogeneous data. We conclude that this visual workflow offers a scalable, data-driven solution for moving from raw, imperfect observations toward actionable system diagnostics, bridging the gap between data acquisition and process understanding in complex environmental observatories.

How to cite: Gutiérrez, K., Lischeid, G., Demir, G., Dubbert, M., Knohl, A., and Markwitz, C.: Unsupervised pattern recognition for imperfect datasets: a visual workflow for plausibility checks and regime diagnosis in high-dimensional environmental time series, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11636, https://doi.org/10.5194/egusphere-egu26-11636, 2026.

EGU26-11928 | Posters on site | HS3.8

A Disjunctive Interpretation Approach to Missing Data Based on Clustering Quality 

hamza khyari and Salem Benferhat

Data completion is a major challenge in many applications, particularly in Geographic Information Systems (GIS) for water networks. Numerous approaches have been proposed to address this problem, ranging from classical statistical methods to artificial intelligence-based techniques.

In this presentation, we address the problem of missing or imprecise data in water network GIS by proposing a clustering-based data completion approach. For a given attribute with missing or uncertain values, each possible value in the attribute domain is considered as a candidate for completion. Each candidate is evaluated by analyzing its impact on the clustering of the entire dataset: inserting a candidate value induces a specific global clustering, whose quality is assessed using appropriate clustering validity criteria. The value that yields the highest-quality clustering, namely the one that best captures the intrinsic structure of the data, is selected as the final completion value.

To cope with the combinatorial explosion resulting from multiple attributes with missing values and large domains, several strategies are employed to reduce the number of candidate completions, including aggregation mechanisms, while maintaining both the effectiveness and efficiency of the proposed approach.

How to cite: khyari, H. and Benferhat, S.: A Disjunctive Interpretation Approach to Missing Data Based on Clustering Quality, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11928, https://doi.org/10.5194/egusphere-egu26-11928, 2026.

EGU26-14633 | Posters on site | HS3.8

Composing Transparent Quality Control Pipelines from Basic Anomaly Descriptions 

Peter Lünenschloß, David Schaefer, and Jan Bumberger

Quality control (QC) and data cleaning remain major bottlenecks in geoscientific data analysis as data volumes, dimensionality, and heterogeneity continue to increase. While machine- and deep-learning-based approaches have demonstrated impressive performance in selected applications, their practical adoption is often constrained by the availability of sufficiently large labelled training datasets and by the effort required to calibrate and adapt model hyperparameters across datasets and domains, particularly in unsupervised flagging scenarios. Conversely, rule-based, deterministic, and statistical QC approaches offer greater transparency and interpretability, but are frequently tailored to specific data structures and lack the flexibility required to robustly generalise to varying observational contexts and non-ideal data distributions.

We present a software framework that addresses this gap by enabling the formulation of QC pipelines in terms of a small set of basic anomaly descriptions, such as outliers, noisy regimes, and data gaps. These anomaly notions are intuitively understood by domain experts, while their systematic combination allows the representation of a wide range of anomaly patterns encountered in geoscientific observations.

The parameters of these compositions are then automatically calibrated with the data at hand, resulting in an instantiated QC pipeline. By internally reducing the calibration problem to the fitting of individual anomaly descriptions defined by only a small number of well-understood parameters, the optimisation achieves robust convergence even with a limited number of supervised examples. Within the framework, such examples can be generated interactively during pipeline construction by domain specialists themselves or imported from existing sources. This design lowers the entry barrier for effective automated quality control while enabling the explicit integration of domain knowledge into the calibration process.

The framework is implemented as a new module within the open-source quality-control software SaQC, thereby integrating seamlessly with existing data import, preprocessing, and flag management workflows. Calibrated QC pipelines can be exported and stored as portable, human-readable configuration files in a tabular format. These configurations can subsequently be loaded and applied using the SaQC application to new and unseen datasets, enabling reproducible and automated quality control.

In the poster, we present the conceptual design of the framework and demonstrate its application to a hydrological dataset, highlighting the transparent, combinatorial configuration interface and the integrated supervision workflow.

 

How to cite: Lünenschloß, P., Schaefer, D., and Bumberger, J.: Composing Transparent Quality Control Pipelines from Basic Anomaly Descriptions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14633, https://doi.org/10.5194/egusphere-egu26-14633, 2026.

EGU26-14708 | ECS | Orals | HS3.8

A Knowledge Graph–Based Approach for reconciling Geological information 

Imadeddine laouici and Fatma Chamekh

The understanding of the subsurface relies on integrating heterogeneous geological information originating from geological maps, geological models, and textual sources such as reports and scientific publications. In current practice, these sources remain rarely homogenized and are reconciled manually by domain experts, mostly in the context of 3D geomodel construction projects. Even when information is reconciled, existing methods offer limited support for expert knowledge integration, traceability of interpretations, and automated wholistic consistency checking.

We propose SemTrack, an ontology-based integration approach designed to formalize, reconcile, and exploit multi-source geological information within a unified knowledge graph. In this framework, SemTrack integrates structured information extracted from maps and numerical geological models with unstructured knowledge derived from textual documents, all aligned through a dedicated modeling ontology. The resulting knowledge graph supports logical reasoning and knowledge inference using SWRL rules to ensure the consistency of geological constraints and allows to explicitly encode expert interpretations record. This enables the automation of conceptual inconsistencies detection, transparent inference of implicit geological relationships, the completion of missing information across multiple sources, and advanced complex querying of initially heterogenous geological information.

How to cite: laouici, I. and Chamekh, F.: A Knowledge Graph–Based Approach for reconciling Geological information, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14708, https://doi.org/10.5194/egusphere-egu26-14708, 2026.

EGU26-15597 | Posters on site | HS3.8

Quality Control of Redundant Water Level Gauges in South Korea River Gauging Stations 

TaeWoong Ok, ChiYoung Kim, KiYong Kim, and ChanWoo Kim

In South Korea, river stage gauging stations operate redundant water level gauges to mitigate instrument malfunctions and anomalous measurements. Currently, redundant gauges are installed at over 60% of gauging stations, reflecting their widespread implementation; however, their quality management and practical utilization remain limited. In many cases, installation and operational conditions are not fully accounted for in observed water levels, leading to significant discrepancies between primary and redundant gauges. These discrepancies may arise from river characteristics, artificial configuration errors, or site-specific conditions.

 

This study investigates the causes of discrepancies between primary and redundant gauges and proposes appropriate correction methods. Anomaly detection was first conducted on redundant gauge measurements using limit tests, duration tests, and regression tests to ensure data reliability. Based on this, the relationships between primary and redundant gauge readings were analyzed using simple regression, multiple regression, and nonparametric LOESS (Locally Estimated Scatterplot Smoothing) regression. These procedures not only facilitated the derivation of site-specific correction methods but also supported the preliminary development of a real-time quality control program, moving beyond conventional manual, non-real-time quality management.

 

Nevertheless, because the causes of discrepancies and installation conditions vary by site, site-specific correction strategies are required, and ongoing monitoring and refinement of measurements and corrections remain necessary. Furthermore, real-time utilization of redundant gauges is challenging at newly established stations. Despite these limitations, the proposed correction strategies have the potential to go beyond simple substitution of primary gauge readings, enabling higher-quality hydrological data production and improved quality control. These strategies are expected to enhance real-time hydrological monitoring systems and strengthen the reliability of national hydrological data management frameworks.

Keywords : Redundant, Water Level Gauging, Uncertainty, Operational Monitoring

 

Acknowledgements

This work was supported by Korea Environment Industry & Technology Institute(KEITI) through Research and Development on the Technology for Securing the Water Resources Stability in Response to Future Change Project, funded by Korea Ministry of Climate, Energy, Environment(MCEE)(RS-2024-00332300).

How to cite: Ok, T., Kim, C., Kim, K., and Kim, C.: Quality Control of Redundant Water Level Gauges in South Korea River Gauging Stations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15597, https://doi.org/10.5194/egusphere-egu26-15597, 2026.

EGU26-15843 | Posters on site | HS3.8

Comparative Evaluation of Daily Streamflow Gap-Filling Using Paired Upstream–Downstream Gauges 

Chi Young Kim, Chanwoo Kim, and Taewoong Ok

Complete daily streamflow time series are essential for sustainable water resources management and reliable hydrological modelling; however, even short data gaps can substantially reduce the usability of streamflow records. Recurrent missing data may lead to inefficient model calibration, decreased reliability of peak and low-flow estimates, and biased hydrological statistics. Therefore, rather than leaving missing values unfilled, it can be beneficial to infill daily streamflow using appropriate methods and to provide flags indicating imputed periods. 
In South Korea, streamflow monitoring prior to 2008 primarily focused on flood-related observations, resulting in relatively limited daily streamflow records; since then, the production of continuous daily streamflow data for water resources management has expanded. As of 2024, daily streamflow records from more than 420 gauging stations are managed and disseminated, yet a non-negligible number of stations still contain missing values due to various causes such as river works and uncertainties in stage–discharge relationships associated with the operation of hydraulic structures. 
This study comparatively evaluates gap-filling techniques using paired upstream–downstream gauging stations located in basins with diverse rainfall regimes and hydrological characteristics. We assess conventional methods widely used in practice (scaling, linear regression, and equi-percentile/quantile-based approaches) under different missing-data conditions and benchmark them against an extended long short-term memory (extended LSTM) time-series model designed for streamflow infilling. Performance is evaluated using the Nash–Sutcliffe efficiency (NSE), root mean square error (RMSE), and percent bias (PBIAS). In addition, flow duration curves (FDCs) are compared to examine each method’s ability to reproduce the post-infilling flow regime distribution. The outcomes are expected to support condition-dependent selection of gap-filling strategies and to improve the reliability of daily streamflow datasets with explicit quality flags.

How to cite: Kim, C. Y., Kim, C., and Ok, T.: Comparative Evaluation of Daily Streamflow Gap-Filling Using Paired Upstream–Downstream Gauges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15843, https://doi.org/10.5194/egusphere-egu26-15843, 2026.

EGU26-17357 | Posters on site | HS3.8

A Preliminary Analysis of High Water Events in Venice Based on Multi-Decadal Observations and Clustering 

Franco Alberto Cardillo, Angela Andrigo, Francesco De Biasio, Franca Debole, Marco Favaro, Alvise Papa, Umberto Straccia, and Stefano Vignudelli

High water events in Venice are a recurrent phenomenon, as the city is located only slightly above mean sea level and is directly influenced by water-level variations within the lagoon. Flooding occurs when several physical processes act in combination. The astronomical tide determines the baseline water level, which is subsequently modulated by seiche oscillations in the Adriatic Sea, meteorological forcing (e.g. wind stress and atmospheric pressure), and slower, low-frequency geophysical processes and sea level rise. When these factors co-occur, even if individually moderate, large portions of the city may experience flooding.

Repeated flooding has significant economic and social impacts, limits pedestrian and naval traffic and contributes to the degradation of buildings and cultural heritage. To mitigate these effects, a range of protective measures is implemented and coordinated by an early warning system. The effectiveness of these measures depends on their timely activation. However, mitigation actions are associated with substantial economic costs and may themselves generate negative impacts if deployed unnecessarily. For instance, interruptions to public transport services affect daily activities, while the operation of the MOSE barrier entails considerable financial costs. Accurate and reliable forecasts are therefore essential to balance flood protection with the economic and social costs of mitigation measures.

Current forecasting systems primarily estimate water levels and peak values, and these are typically estimated at a limited number of locations. These systems are based on sophisticated statistical and hydrodynamic models. Although they perform well in most situations, their accuracy can be affected by uncertainties in atmospheric forcing and by limitations in representing the full variability of high water events. This work explores the potential of complementary approaches based on the analysis of observational data rather than explicit physical modelling.

Data-driven approaches, in particular Machine Learning (ML) methods, analyze historical data without relying on predefined, human-designed model structures. ML models are able to capture recurring patterns and complex feature interactions that are difficult to incorporate into traditional numerical models. Among these approaches, clustering techniques aim to identify recurrent types of events based on similarities in their temporal evolution and associated meteorological conditions. This enables events characterized by similar water levels to be differentiated according to the combinations of underlying meteorological drivers, thereby providing additional information to support forecasting and response planning.

In this work, we present a preliminary analysis based on several clustering approaches, including k-means, DBSCAN, and deep learning–based methods, applied to a multi-decadal atmospheric dataset and to the longest available reconstructed hourly sea-level records for the northern Adriatic Sea, specifically developed for this study. We compare the resulting event classifications and discuss how cluster-derived information may complement existing forecasting systems in support of flood-mitigation strategies for the city of Venice.

How to cite: Cardillo, F. A., Andrigo, A., De Biasio, F., Debole, F., Favaro, M., Papa, A., Straccia, U., and Vignudelli, S.: A Preliminary Analysis of High Water Events in Venice Based on Multi-Decadal Observations and Clustering, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17357, https://doi.org/10.5194/egusphere-egu26-17357, 2026.

Managing multi-source data requires flexible approaches and tools to model many types of imperfections surrounding them and, and more braodly, to deal with uncertainties of multiple origins, namely aleatory (representing randomness) and epistemic uncertainty (related to imperfect knowledge). While the first origin can be adequately represented using classical probabilities, there is no simple, single answer for epistemic uncertainty. New theories of uncertainty based on "imprecise probabilities" have been developed in the literature to go beyond the systematic use of a single probabilistic law. In this communication, I analyze the application of these methods for quantifying uncertainty in various real-world cases of natural hazard assessment (earthquakes, floods, rockfalls) in terms of their advantages and disadvantages compared to the traditional probabilistic approach. On this basis, I draw lessons to support decision making under uncertainty and identify open questions and remaining challenges, in particular the integration of spatio-temporal geodata, the use of full process high-fidelity numerical models, and interfacing with AI-based approaches.

I acknowledge financial support of the French National Research Agency within the HOUSES project (grant N°ANR-22-CE56-0006).

How to cite: Rohmer, J.: Dealing with imperfect knowledge in natural hazard assessments: beyond classical probabilities and challenges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17687, https://doi.org/10.5194/egusphere-egu26-17687, 2026.

EGU26-19993 | ECS | Orals | HS3.8

Uncertainty produced in a 15-minute gridded rainfall product for the UK.  

Tom Keel, Matt Fry, and Sam Counsell

Reliable rainfall datasets are an essential foundation for hydrological research. The most extensive rainfall information is collected from rain gauge networks, which provide high-frequency observations on rainfall intensity at those locations, or their data can be interpolated onto a regular grid to provide consistent region-wide estimates.

For the UK, there are two major daily gridded rainfall products: (1) CEH-GEAR developed by the UK Centre for Ecology & Hydrology, and (2) HadUK-Grid developed by the Met Office. In each case, they are built from a selection of rain gauges from a multi-nation rain gauge network spanning Great Britain. Decisions made at each stage of rainfall data preparation, about collection, formatting, quality control and then gridding, introduce uncertainty into the resulting gridded rainfall products.

In this talk, we discuss plans for CEH-GEAR 15 min, a new sub-daily 1 km product developed as part of the UK’s multi-year Flood & Drought Research Infrastructure (FDRI) project. We detail each step of its production, from raw rain gauge to gridded rainfall estimates, and systematically discuss the sources of uncertainty introduced at each stage. 15-minute rainfall measurements tend to be highly variable in space and time, and intense storms or long dry periods create practical challenges for preparing gridded rainfall estimates. So, we quantify the sensitivity of those estimates to decisions made about quality control and data blending during notable rain events across the UK. We also present the associated open-source tools developed as part of FDRI, including RainfallQC, that aim to support reproducible rainfall data processing and alleviate some of the challenges in sub-daily rainfall data preparation.

How to cite: Keel, T., Fry, M., and Counsell, S.: Uncertainty produced in a 15-minute gridded rainfall product for the UK. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19993, https://doi.org/10.5194/egusphere-egu26-19993, 2026.

EGU26-23039 | Posters on site | HS3.8

Managing Incomplete Urban Reference Data for Risk-Oriented Geoscience Applications: Lessons from the CERES Project 

Gracianne Cécile, Youssef Fouzai, Mirga Bokidingo, Caterina Negulescu, Yves Lucas, Gilles Grandjean, and Fatima Chamekh

Assessing exposure and vulnerability to natural hazards increasingly relies on national geospatial reference datasets. However, these datasets are often incomplete, heterogeneous and inconsistent across spatial scales, which limits their direct usability for multi-hazard risk analysis. In France, the BD TOPO building database exemplifies these challenges, with a large share of buildings lacking key attributes such as usage type, despite their importance for vulnerability assessment.
This contribution presents the approach developed within the CERES project (Cartography and Characterization of Exposed Elements from Satellite Imagery) to address reference data incompleteness and multi-source integration challenges in a geoscience risk context. Focusing on a large study area in the Centre-Val de Loire region, we first quantify and analyze the spatial and semantic gaps of BD TOPO building attributes, showing that more than 40% of buildings are labelled with unknown usage. We then demonstrate how deep learning applied to very high-resolution aerial imagery can be used to probabilistically infer missing semantic information, significantly reducing uncertainty while explicitly accounting for classification ambiguities.
Beyond data completion, we highlight the difficulties encountered when jointly exploiting heterogeneous datasets originating from national mapping agencies, land cover products, socio-economic statistics and hazard layers. These include spatial misalignments, inconsistent scales of representation, varying levels of reliability, and the absence of a shared data model. To address these issues, CERES proposes a multi-scale data structuring framework combining data modelling and processing designed to preserve data provenance, uncertainty and semantic traceability across sources.
By articulating reference data analysis, machine-learning-based enrichment and database design, this work provides a concrete illustration of current practices and challenges in managing imperfect geospatial data for geoscience applications. The results underline the necessity of coupling data-driven approaches with explicit data governance and modelling strategies to produce robust, transparent and reusable datasets for territorial risk assessment.

How to cite: Cécile, G., Fouzai, Y., Bokidingo, M., Negulescu, C., Lucas, Y., Grandjean, G., and Chamekh, F.: Managing Incomplete Urban Reference Data for Risk-Oriented Geoscience Applications: Lessons from the CERES Project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23039, https://doi.org/10.5194/egusphere-egu26-23039, 2026.

GI3 – Planetary Atmosphere and Ocean instrumentation system

EGU26-1113 | ECS | Orals | PS7.2

The effect of present-day mantle temperature anomalies on crustal thickness inversions for the Moon 

Sabatino Santangelo, Ana-Catalina Plesa, Adrien Broquet, Doris Breuer, and Matthias Grott

Considering a laterally variable crustal thickness has important effects on modeling the 3D geodynamical evolution of terrestrial bodies (e.g., Plesa et al., 2016; Fleury et al., 2024; Santangelo et al., 2025). On the one hand, it provides an orientation for the geodynamic model by correlating subsurface regions with surface features such as craters and volcanic centers. On the other hand, it improves the geodynamic model, allowing it to capture temperature fluctuations induced by thickness variations in a radiogenically enriched and low-conductivity crust.

Asymmetries in the subsurface temperature predicted by geodynamical models at present-day will induce gravity field anomalies that can, in turn, affect crustal thickness inversions. In the case of the Moon, a present-day thermal asymmetry between near- and far-side has been predicted by several studies (e.g., Laneuville et al., 2013, 2018; Park et al., 2025; Santangelo et al., 2025), possibly induced by the concentration of radioactive isotopes underneath the nearside crust. This 100–200 K temperature anomaly in the mantle translates to a large-scale and prominent negative density anomaly, which is yet to be accounted for by inversions of gravity data for the crustal thickness of the Moon (e.g., Wieczorek et al., 2013).

In this work, we couple geodynamic models together with gravity and topography inversions of crustal thickness to provide self-consistent estimates of the lunar mantle and crustal structure. We convert subsurface thermal anomalies predicted by the thermal evolution model into density anomalies using a pressure- and temperature-dependent parameterization of the thermal expansivity (Tosi et al., 2013). The density anomalies are used as input to invert for the crustal thickness distribution. The crustal thickness inversion model used in this study has been adapted from the setup described in Broquet et al., (2024). 

For self-consistency, we iterate between the crustal thickness and the geodynamic model, as the density anomalies obtained in the geodynamic model result from crustal thickness variations and associated distribution of radiogenic isotopes, while the crustal thickness inversion itself depends on the density anomalies and associated density contrast at the crust-mantle boundary. Convergence is reached within a couple of iterations. 

We find that a positive temperature anomaly associated with the enrichment of radiogenic isotopes beneath the lunar near side, as required to explain the Apollo 15 and Apollo 17 heat flux measurements (Langseth et a., 1976), induces a crustal thinning up to 8.5 km in the Procellarum KREEP Terrane (PKT) region. Conversely, the positive density anomaly associated with a colder lunar interior underneath the thin-crust South-Pole Aitken basin produces a crustal thickening of ~3 km.

Our coupled geodynamic crustal thickness models show that the effects of subsurface temperature anomalies can lead to changes in crustal thickness estimates comparable to the uncertainty in the seismically derived crustal thickness measurements (~8 km; Chenet et al., 2006). Thus, considering temperature anomalies on crustal thickness modeling has important implications for our understanding of the crustal structure of the Moon. Upcoming seismic and heat flow measurements will, therefore, be critical to discriminate between different interior structure models. 

How to cite: Santangelo, S., Plesa, A.-C., Broquet, A., Breuer, D., and Grott, M.: The effect of present-day mantle temperature anomalies on crustal thickness inversions for the Moon, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1113, https://doi.org/10.5194/egusphere-egu26-1113, 2026.

EGU26-1845 | ECS | Orals | PS7.2

Magnetic characterisation of volcanic rocks from the Tajogaite eruption. 

Ángel Melguizo Baena, Miguel Ángel Rivero Rodríguez, Alberto López Escolano, Sergio Fernández Romero, Leonardo Ntelakrous Karnavas, Joana S. Oliveira, and Marina Díaz Michelena

The Tajogaite eruption provides a recent example of the construction of a volcanic edifice and an opportunity to track the evolution of the volcano and its products. The eruption was active from 19 September to 13 December 2021, making its surface incursion into the Cumbre Vieja volcanic rift. Over the months, there were several eruptive vents that built a main edifice. Among its main products were tephritic and basanitic lava flows, some reaching the coast; pyroclastic materials near the cone, such as bombs; and ash ejection throughout the process.

The aim of this work is to study the mineralogical composition through the magnetic characterisation of the rocks. The lavas from the 2021 eruption have similar compositions, ranging from tephrites to basanites, emitted in the early and late stages of the eruption, respectively, with the former being richer in amphibole and the latter richer in olivine. Rocks emitted by the Tajogaite volcano are compared with those from other eruptions on the island, such as San Juan (1949) and Tacande (1480).

To this end, a methodology is employed which consists, firstly, of collecting field samples for magnetic characterisation. With the aid of a Vibrating Sample Magnetometer, the natural remanence of the samples, the first magnetisation curves and the hysteresis loops are measured.

An original contribution of this work is the use of a normalisation of the first magnetisation curves. Depending on their shape and changes in slope, compositional differences in the samples can be identified due to variations in their magnetic carriers. Therefore, we associate different curves with different rock compositions.

How to cite: Melguizo Baena, Á., Rivero Rodríguez, M. Á., López Escolano, A., Fernández Romero, S., Ntelakrous Karnavas, L., Oliveira, J. S., and Díaz Michelena, M.: Magnetic characterisation of volcanic rocks from the Tajogaite eruption., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1845, https://doi.org/10.5194/egusphere-egu26-1845, 2026.

EGU26-3345 | Posters on site | PS7.2

Exploration of Degree-1 Heterogeneities in the Lunar Mantle Using CitcomSVE 

Alex Guinard, Javier Abreu-Torres, Agnès Fienga, Shijie Zhong, and Anthony Mémin

Recent reprocessing of NASA's GRAIL mission gravimetric data in the work of Park et al. (2025) allowed for the estimation of the third-degree lunar tidal Love number, k3, at a monthly tidal period of 27.3288 days. The obtained value, k3 = 0.0163 ± 0.0007, is significantly higher than predictions based on spherically symmetric models of the lunar interior. This same study suggests that this high k₃ value could be explained by the presence of a degree-1, order-1 anomaly in the lunar mantle shear modulus, with an amplitude of approximately 3%.

In this work, we investigate the tidal response of laterally heterogeneous lunar interiors using 3-D viscoelastic modeling and considering not only elastic framework but also viscoelastic rheology. Using CitcomSVE – a finite-element code initially developed for modeling glacial isostatic adjustment deformations – we model the lunar interior as suggested in the results of Park et al. (2025), i.e., for degree-1, order-1 mantle anomaly in shear modulus. We further quantify tidal dissipation at both monthly and yearly (365.260 days) forcing periods to assess whether the dissipation predicted by this model is consistent with current observational constraints on lunar tidal dissipation.

How to cite: Guinard, A., Abreu-Torres, J., Fienga, A., Zhong, S., and Mémin, A.: Exploration of Degree-1 Heterogeneities in the Lunar Mantle Using CitcomSVE, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3345, https://doi.org/10.5194/egusphere-egu26-3345, 2026.

EGU26-3738 | Posters on site | PS7.2

Composition and Provenance of the Chang’e-4 Landing Area 

Hongbo Zhang, Dawei Liu, Zhibin Li, Zongyu Zhang, and Chunlai Li

This study systematically analyzes the composition and origin of materials in the Chang’e-4 landing area (Von Kármán crater) using 131 in-situ lunar soil spectra from the first 60 lunar days obtained by Visible and Near-infrared Imaging Spectrometer onboard Yutu-2 rover and spectral data from the Moon Mineralogy Mapper (M3). Results show that the 2μm absorption center of the landing area aligns with that of Finsen ejecta, while the 1μm absorption center shifts toward longer wavelength, suggesting an enrichment in olivine or glass of the landing area. The surface materials at the landing area might originate from the distal ejecta of Finsen crater.

Based on the Chang'e-2 Digital Orthophoto Map(DOM) data and the geological characteristics along the traverse area of Yutu-2 rover, we found that the rock types in and around the Von Kármán crater can be classified into three categories. (1)Basalts formed in two different periods. The late-stage basalt is flood lava (approximately 320m thick), originating from Leibniz crater. The old basalts represent the basement rock at the bottom of Kármán crater; (2)Widely distributed weathered deposits. Although their spectra are similar to those of Finsen ejecta, these deposits are located at the distal end of the ejecta rays, exhibit variable thickness, and reveal local fragmented blocks beneath them. This suggests that the deposits likely represent a mixture of ejecta material and local substrate; (3) Highland rocks. The basement rocks that predate the Von Kármán and Von Kármán M craters are represented by a large number of highland rocks, which form the rim plateau around the Von Kármán crater. The distal position and heterogeneous thickness of the Finsen ejecta at the landing area indicate that the Finsen-forming impact event only modified the composition of landing area surface regolith at millimeter- to centimeter-scale depths, without causing significant topographic alteration.

How to cite: Zhang, H., Liu, D., Li, Z., Zhang, Z., and Li, C.: Composition and Provenance of the Chang’e-4 Landing Area, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3738, https://doi.org/10.5194/egusphere-egu26-3738, 2026.

EGU26-3845 | ECS | Orals | PS7.2

On the Crustal Architecture of the Terrestrial Planets 

Adrien Broquet, Julia Maia, and Mark A. Wieczorek

The crust is the outermost solid layer of a rocky body with a composition that substantially differs from the deeper interior (mantle and core). Due to its lower thermal conductivity, the crust thermally insulates the interior, and thus the thickness of the crust controls the rate at which a planet cools in time (Plesa et al., 2022). The crust preserves a record of a planet’s geologic history, hosting remanent magnetization from interior dynamos (e.g., Langlais et al., 2010), and has been scarred by tectonic (e.g., Andrews-Hanna & Broquet, 2023), impact (e.g., Melosh et al., 2013), volcanic (e.g., Carr & Head, 2010) and erosional processes (e.g., Hynek et al., 2010). For these reasons, understanding the structure and composition of the crust is fundamental for uncovering the diverse geologic pathways of rocky bodies in the solar system.

In this work, we provide a broad overview of our current knowledge of the composition and structure of planetary crusts following Broquet et al. (2025). We summarize the different geophysical approaches to characterize the shape of the crust and propose improvements to existing inversions of observed gravity and topography for crustal thickness from both conceptual and theoretical perspectives. In particular, we discuss how the gravity field resolution, data filtering, crustal density as well as the elastic and dynamic support of topography all affect crustal thickness inversions. Based on these improvements, we propose refined crustal thickness models for Mercury, Venus, Mars, and the Moon.

Andrews-Hanna, J.C., & Broquet, A. (2023). The history of global strain and geodynamics on Mars. Icarus 395. doi: 10.1016/j.icarus.2023.115476.

Broquet, A., Maia, J., & Wieczorek, M.A. (2025). On the crustal architecture of the terrestrial planets. J. Geophys. Res. Planets 130, e2025JE009139. doi: 10.1029/2025JE009139

Carr, M.H., & Head, J.W. (2010). Geologic history of Mars. Earth Planet. Sci. Lett. 294. doi: 10.1016/j.epsl.2009.06.042.

Hynek, B.M., Beach, M., Hoke, M.R. (2010). Updated global map of Martian valley networks and implications for climate and hydrologic processes. J. Geophys. Res. Planets 115(E9). doi: 10.1029/2009JE003548.

Langlais, B., Lesur, V., Purucker, M. et al. (2010). Crustal Magnetic Fields of Terrestrial Planets. Space Sci. Rev. 152, 223–249. doi: 10.1007/s11214-009-9557-y.

Melosh, H.J., Freed, A.M., Johnson, B.C., et al. (2013). The Origin of Lunar Mascon Basins. Science 340. doi: 10.1126/science.1235768.

Plesa, A.-C., Wieczorek, M.A., Knapmeyer, M., Rivoldini, A., Walterová, M., Breuer, D. (2022). Chapter Four - Interior dynamics and thermal evolution of Mars - a geodynamic perspective. Adv. Geo. 63. 10.1016/bs.agph.2022.07.005.

How to cite: Broquet, A., Maia, J., and Wieczorek, M. A.: On the Crustal Architecture of the Terrestrial Planets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3845, https://doi.org/10.5194/egusphere-egu26-3845, 2026.

EGU26-6046 | Orals | PS7.2

Synchronisation of the Pluto-Charon binary by inward tidal migration. 

Michael Efroimsky, Michaela Walterova, Yeva Gevorgyan, Amirhossein Bagheri, Valeri V. Makarov, and Amir Khan

The dwarf planet Pluto and its largest moon Charon represent a fully tidally evolved system: their orbital eccentricity is almost zero and their respective rotational periods are equal to the mutual orbital period. According to a widely accepted hypothesis, Charon as well as other Pluto moons originated in a giant oblique impact (e.g., Canup et al., 2005; Arakawa et al., 2019), forming on a tight orbit above the synchronous radius, and evolved by tidal recession from the primary, which was endowed with a large angular momentum and thus fast rotation. A recent, alternative scenario proposes formation by collisional capture (Denton et al., 2025), resulting in Charon’s emplacement on an initially circular close-in orbit and a primordial synchronisation at high spin rate.

A tidally evolving binary is subjected to surface stresses that are strongly dependent on the mutual distance and, for small orbital separations, may lead to the formation of tidally-oriented fractures in the ice shell similar to those on Enceladus or Europa. The orientation of fractures identified on images from the New Horizons mission is, however, not correlated with expected tidal stresses and has instead been attributed to ocean freezing, which would have postdated the full orbital evolution (Rhoden et al., 2020). Moreover, an initially quickly rotating Pluto (and Charon) consistent with the giant impact scenarios would lead to a considerable rotational bulge that would only be able to relax before present in the case of a thin lithosphere and a weak ice shell above a subsurface ocean (McKinnon et al., 2025).

Here, we present a model of the Pluto-Charon synchronisation that predicts lower tidal stresses and does not require initial fast rotation of the partners, thus potentially alleviating some of the challenges posed by the standard tidal recession scenario. We propose that the binary was formed by a capture of a highly inclined retrograde minor planet (proto-Charon) by a prograde-rotating Pluto and subsequently evolved by tidal approach. Following this line, we perform numerical simulations of the binary’s orbital evolution, studying the effect of various initial spin rates, eccentricities, and interior properties. During the evolution, Pluto acquires its present-day retrograde rotation and, depending on ice viscosity, Charon may experience episodes of higher spin-orbit resonances (such as 3:2 or 2:1). Since the evolution of a planet with a retrograde moon proceeds at distances greater than the present-day semi-major axis, both Pluto and Charon experience tidal heating and stresses two orders of magnitude lower than in the tidal recession scenario.

How to cite: Efroimsky, M., Walterova, M., Gevorgyan, Y., Bagheri, A., Makarov, V. V., and Khan, A.: Synchronisation of the Pluto-Charon binary by inward tidal migration., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6046, https://doi.org/10.5194/egusphere-egu26-6046, 2026.

EGU26-10257 | ECS | Posters on site | PS7.2

Computing the size of Mercury’s impact basins and ring systems through gravity data modelling 

Salvatore Buoninfante, Mark A. Wieczorek, Valentina Galluzzi, Gene W. Schmidt, and Pasquale Palumbo

Impact basins on terrestrial planets have been thoroughly investigated from imagery and topography data. Previous work has already shown the presence of peak-ring basins on terrestrial planets and estimated their size (e.g., [1]), utilising topography and morphological data. However, the modelling of gravity and crustal thickness data can be a powerful approach in detecting hidden impact basins and estimating the diameters of their rim and inner rings. This is also useful in updating the basin catalogue of terrestrial planets and provides valuable constraints to accurately estimate the impact rate during the early Solar System.

NASA’s MESSENGER mission provided most datasets used in the last decade to model the internal structure of Mercury and characterize its surface. Image products derived after MESSENGER have been widely used to detect impact basins and provide a consistent database [2, 3]. More recently, Mercury’s gravity anomalies have also been used to re-update this catalogue [4].

Here we model Bouguer gravity anomalies of Mercury using the MESS160A gravity field model [5] to properly estimate the size of inner rings. We first quantify a regional value of the Bouguer gravity anomaly, which is defined as the average value obtained from azimuthally averaged profiles in the spatial range 1.5D to 2D, where D is the basin diameter. The size of the Bouguer gravity high is derived as the radius where the profiles first intersect the regional values. The uncertainties represent the ±1σ values of the regional values taken in the same spatial range. We performed tests on filtered GRAIL gravity data, consistently with the spatial resolution of Mercury’s gravity field, to understand how the resolution affects the size estimates of certain lunar basins [6]. The used approach can be reliable for inner ring diameters ≳ 70 km when considering the highest gravity resolution for Mercury.

We present preliminary results for selected certain impact basins [2, 3, 7] in the northern hemisphere where the current gravity data is characterized by higher resolution, and for putative or uncertain basins [2, 3]. The results confirm the existence of the investigated certain and putative basins, and provide updated inner ring sizes.

This approach will be first used to identify potential unknown impact basins, re-evaluate the existing databases of impact basins on Mercury, and it can be valuable in assessing the existence and number of multi-ring basins on Mercury. Though our current database focuses on basins in the northern hemisphere, the approaching ESA-JAXA BepiColombo mission will provide higher-resolution gravity data in the southern hemisphere, allowing us to better quantify the impact basins size at these latitudes.

References

[1] Baker D. M. H. et al. (2011). Planet. Space Sci., 59(15).

[2] Fassett C. I. et al. (2012). JGR: Planets, 117(E12).

[3] Orgel C. et al. (2020). JGR: Planets, 125(8).

[4] Szczech C. C. et al. (2024). Icarus, 422.

[5] Konopliv A. S. et al. (2020). Icarus, 335.

[6] Neumann, G. A. et al. (2015). Sci. Adv., 1(9).

[7] Hall G. P. et al. (2021). JGR: Planets, 126(9).

 

Acknowledgements: We gratefully acknowledge funding from the Italian Space Agency (ASI) under ASI-INAF agreement 2024-18-HH.0.

How to cite: Buoninfante, S., Wieczorek, M. A., Galluzzi, V., Schmidt, G. W., and Palumbo, P.: Computing the size of Mercury’s impact basins and ring systems through gravity data modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10257, https://doi.org/10.5194/egusphere-egu26-10257, 2026.

EGU26-13434 | Orals | PS7.2

Lunar Optical Very Broad Band: a high-performance seismometer for Moon deep interior study 

Sebastien de Raucourt, Frédéric Guattari, Gabrielle Chabaud, Mélanie Drilleau, Taichi Kawamura, Philippe Lognonné, Tanguy Nebut, Olivier Robert, and Sylvain Tillier

More than 50 years after Apollo, the Moon deep interior structure is still not well known. Several seismic experiments are expected on the Moon surface in the coming year (Chang’e 7, Chandrayan, Artemis III, FSS and SPSS). All of those seismometers are not expected to resolved the seismic background of the Moon and their performances are not meeting the International Lunar Network requirements (10-11 m.s-2/sqrt(Hz)).

To meet this requirement, IPGP is developing an optical seismometer operated in open loop. Its mechanical oscillator is a 1Kg proof mass suspended by a 4 cross blades hinge and a leaf spring with extremely low damping. Its displacement sensor is a Michelson interferometer, associated to a narrow bandwidth laser source and an optical phase readout electronic inherited from fiber optics gyroscope. This instrument will be candidate for all flight opportunities around 2030 (launch date).

The first prototypes performances tests demonstrated the potential of this technology. But it also revealed that stray light inside the interferometer is limiting its performance. Different techniques of characterization of the stray light are compared: in situ coherent detection, characterization using a delay line and short coherency length light source. Tests results are compared to simulation.

Analysis of the stray light impact on the performances through the optical phase readout electronic modulation scheme shows the impact on performances. Expectation and performances potential of the next prototypes generation is discussed.

How to cite: de Raucourt, S., Guattari, F., Chabaud, G., Drilleau, M., Kawamura, T., Lognonné, P., Nebut, T., Robert, O., and Tillier, S.: Lunar Optical Very Broad Band: a high-performance seismometer for Moon deep interior study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13434, https://doi.org/10.5194/egusphere-egu26-13434, 2026.

EGU26-13716 | ECS | Orals | PS7.2

Detection and characterization of the Naturalistas and Tahiche lava tubes (Lanzarote, Canary Islands) using vector fluxgate and scalar magnetometer measurements 

Juan Martin de Blas, Yasmina M. Martos, Jared Espley, Dave Sheppard, Stephen Scheidt, Jacob Richardson, and John Connerney

Lava tubes and other subsurface cavities represent key targets for planetary exploration, as they could provide shelter from radiation for astronauts during future exploration missions and are high-priority astrobiology sites. While these structures have been identified on Mars and the Moon, characterization requires conducting geophysical surveys that may first be proven on terrestrial analogs. Among available geophysical methods, magnetic surveys using aerial platforms (e.g., drones or helicopters) offer a cost-effective and easily deployed approach.


The island of Lanzarote (Canary Islands, Spain) is renowned for its volcanic structures—including volcanoes, calderas, and lava tubes—similar to those found on other planetary bodies, particularly Mars. In May 2023, the NASA Goddard Instrument Field Team acquired vector fluxgate and scalar magnetic measurements over three lava tubes in Lanzarote: La Corona, Los Naturalistas, and Tahiche. Previous analyses of the data collected over the Corona lava tube demonstrated the feasibility of using fluxgate magnetic measurements to detect and characterize subsurface cavities. This study focuses on the Naturalistas and Tahiche tubes, which are significantly shallower, shorter, and narrower than La Corona. Specifically, Tahiche exhibits a complex geometry with abrupt changes in size and trajectory. These varied tube geometries provide complementary case studies for validating magnetic surveys for cavity detection, a critical step before conducting magnetometer surveys on other planetary bodies.


We processed our measurements and calculated magnetic anomalies of both the total magnetic field and each of the fluxgate Cartesian vector components. We also applied several enhancement techniques to constrain the location, size, and depth of the two lava tubes. Lastly, we built 2D magnetic forward models for each magnetic transect to reconstruct the geometry and trajectory of the Naturalistas and Tahiche tubes using magnetic data alone. Those geometries will be compared with LiDAR data collected from the tube interiors during the same field campaign. These results provide important guidelines for designing future magnetic surveys on the surfaces of Mars and Moon.

How to cite: Martin de Blas, J., Martos, Y. M., Espley, J., Sheppard, D., Scheidt, S., Richardson, J., and Connerney, J.: Detection and characterization of the Naturalistas and Tahiche lava tubes (Lanzarote, Canary Islands) using vector fluxgate and scalar magnetometer measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13716, https://doi.org/10.5194/egusphere-egu26-13716, 2026.

EGU26-15443 | ECS | Orals | PS7.2

Refining Mercury's tidal Love number h2 through self-registration of MESSENGER laser profiles 

Haifeng Xiao, Attilio Rivoldini, Alexander Stark, Antonio Genova, Tommaso Torrini, Arthur Briaud, Nicola Tosi, Simone Andolfo, Tim Van Hoolst, Hauke Hussmann, Luisa Lara, and Pedro Gutiérrez

Mercury experiences periodic radial surface deformation, quantified by the Love number h2, due to tidal forces exerted by the Sun. Existing measurements come from processing of the Mercury Laser Altimeter (MLA ) profiles using independent approaches: (1) the cross-over analysis (1.55±0.65; Bertone et al., 2021), the self-registration techniques (0.92±0.58; Xiao et al., 2025), and (3) the direct altimetry (1.05±0.29; Stenzel et al., 2025). Unfortunately, the associated uncertainties are still too large to offer meaningful insights into Mercury’s interior (Stenzel et al., this meeting).   

We base our study on Xiao et al. (2025a), but focus on a more polar region of 80°N to 84°N. We permit more reference profiles during the self-registration iterations, adopt higher spatial resolution for the reference terrain model, and minimize projection-induced distortions. To improve the geolocation of MLA footprints, we refine the MESSENGER orbits by carefully modeling non-conservative forces experienced by the spacecraft (Andolfo et al., 2024). Trajectory uncertainty stability is assessed using two independent precise orbit determination frameworks, based on the GEODYN II and MONTE software, respectively. 

The derived tidal deformation time series are shown in Figure 1 and their general trends resemble well that of the tidal signal. After removing the outliers, the inverted tidal h2 converges to between 1.3 and 1.4. Bootstrappings by subsamplings and perturbations considering measurement errors indicate a 3-sigma uncertainty of around 0.1.   

Figure 1. Measured radial tidal deformation against Mercury's mean anomaly (black dots). Theoretical tidal deformation is shown for comparison (blue curves). 

We use the Markov Chain Monte Carlo (MCMC) to infer plausible Mercury interior structure that are consistent with the measured annual libration (Xiao et al., 2025b), tidal Love number k2 (Konopliv et al., 2020), and polar Moment of Inertia (Bertone et al., 2021).  We assume a forsterite/enstatite mantle and a Fe-S-Si core, and consider pressure/temperature dependent properties of the materials. Besides, we take into account the gravitational-pressure couplings at the layer boundaries when estimating the annual libration (Rivoldini and Van Hoolst, 2013). The tidal h2 prediction is around 0.9, which is much smaller than our measurement. 

Currently, we are examining factors that may possibly bias our estimate. We should also note that the study region is extremely limited to within the northern smooth plains which are caused by massive flood volcanism in the past. The large tidal h2 may point to lingering interior heterogeneties, for example, a softer or warmer mantle beneath. 

These activities also stand as a preparation for the upcoming data collected by the BepiColombo Laser Altimeter (BELA) onboard ESA/JAXA’s BepiColombo mission to Mercury (Hussmann and Stark, 2020).  

Acknowledges

AG acknowledges the California Institute of Technology (Caltech) and the Jet Propulsion Laboratory (JPL) for the license of the software MONTE Project Edition. 

References 

Andolfo et al., 2024. JGCD, 47(3), 518-530. Bertone et al., 2021. JGR: Planets, 126(4), e2020JE006683. Hussmann and Stark, 2020. EPJ ST, 229(8), 1379-1389. Konopliv et al., 2020. Icarus, 335, 113386. Rivoldini and Van Hoolst, 2013. EPSL, 377, 62-72. Stenzel et al., 2025. Authorea Preprints. Xiao et al., 2025a. GRL, 52(7), e2024GL112266. Xiao et al., 2025b. EPSC-DPS2025-325. 

How to cite: Xiao, H., Rivoldini, A., Stark, A., Genova, A., Torrini, T., Briaud, A., Tosi, N., Andolfo, S., Van Hoolst, T., Hussmann, H., Lara, L., and Gutiérrez, P.: Refining Mercury's tidal Love number h2 through self-registration of MESSENGER laser profiles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15443, https://doi.org/10.5194/egusphere-egu26-15443, 2026.

EGU26-15471 | ECS | Orals | PS7.2

The Lopsided Moon: Tidal Signals of a Heterogeneous Interior 

Nick Wagner, Alexander Berne, Harriet Lau, and Neal Frankenberg

In the absence of structural asymmetry, the lunar tidal Love numbers should be order independent. Through careful analysis of GRAIL’s non-static gravity field, a recent study by Park et al. (2025; Nature) extracted statistically different ordered Love numbers for the monthly Moon tides, indicative of large scale laterally varying internal structure. In their study, they inverted for variations in shear modulus within the lunar mantle and interpreted these variations in the context of temperature variations. In a complementary, though distinct vein, we jointly invert these new Love numbers, augmented with the same Love numbers for the yearly tides, in tandem with the free-air gravity field and the center-of-mass to center-of-figure offset, to produce a long-wavelength tomographic model of the Moon’s mantle density, elastic, and anelastic properties. To do this, we adapted a normal mode perturbation theory able to predict tidal deformation derived for the Earth that incorporates the Moon's rotation, lateral variations in density, shear and bulk moduli, attenuation, and boundary topography such as the crustal-mantle interface and the core-mantle boundary (Lau et al., 2015; GJI). Since we self-consistently solve for density, shear modulus and attenuation, we are able to interpret our results in the context of both temperature and compositional variations, finding a lower contribution to variations in temperature than in Park et al.’s work and independent density variations within the nearside-farside mantle asymmetry.

How to cite: Wagner, N., Berne, A., Lau, H., and Frankenberg, N.: The Lopsided Moon: Tidal Signals of a Heterogeneous Interior, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15471, https://doi.org/10.5194/egusphere-egu26-15471, 2026.

EGU26-16091 | Orals | PS7.2 | Highlight

The South Pole-Aitken basin constrains the early evolution and differentiation of the Moon 

Jeffrey C. Andrews Hanna, Gabriel Gowman, Shigeru Wakita, Brandon C. Johnson, Amanda Alexander, Carys A. Bill, William F. Bottke, Adrien Broquet, Gareth S. Collins, Thomas M. Davison, Alexander J. Evans, James T. Keane, Janette N. Levin, Ananya Mallik, Simone Marchi, Daniel P. Moriarty III, Samantha A. Moruzzi Fresenius, and Arkadeep Roy

The South Pole-Aitken basin (SPA) is the oldest and largest known impact basin on the Moon.  We use gravity, topography, and surface remote sensing data together with impact simulations to reveal new details of the structure and formation of the basin and to place new constraints on the structure, differentiation, and early evolution of the Moon. The geophysical expression of SPA reveals an elongated, tapered basin formed in a southward-directed oblique impact. Impact simulations show that the downrange excavation from the core of a differentiated impactor can explain the tapered shape of the basin. Remote sensing reveals an asymmetric ejecta blanket rich in thorium, consistent with asymmetric excavation of late-stage lunar magma ocean liquids enriched in incompatible elements such as potassium, rare earth elements, and phosphorus (KREEP). The distribution of Th-rich ejecta can be explained in the context of models of magma ocean crystallization, in which progressive solidification of the magma ocean caused it to become concentrated beneath regions of thinner crust, eventually pinching out to zero thickness beneath the farside highlands and finally concentrating within the nearside Procellarum KREEP terrane.  At an intermediate stage, a thin and discontinuous layer of late-stage magma ocean liquids would have been present beneath the southwestern half of the basin extending onto the nearside, which explains the observed distribution of Th-rich SPA ejecta. Material excavated by SPA on the farside and the younger Imbrium basin on the nearside reveal the evolution of the late-stage magma ocean products in space and time. The ages of these basins and Th concentrations of their ejecta match the modeled compositional evolution of the magma ocean.  Thus, the ejecta of SPA provides a means to sample the late-stage magma ocean as well as the lunar mantle.  High-resolution gravity data reveals an annulus of large-amplitude, short-wavelength gravity anomalies surrounding the basin, consistent with the predicted distribution of material excavated from the lunar mantle. Remote sensing observations of craters excavating into this material indicate a heterogeneous mantle at the time of impact, containing both orthopyroxene-rich and clinopyroxene-rich material. Experimental work predicts that these distinct compositions should form early and late in the magma ocean crystallization sequence, respectively. Thus, the observed compositions are consistent with partial or ongoing overturn of the lunar mantle at the time of the SPA impact. Together, these analyses show how the Moon’s oldest known impact basin provides a key constraint on the interior structure, differentiation, and early evolution of the Moon.  This work provides context for recent, ongoing, and future missions exploring the lunar farside that offer the opportunity for in situ exploration of materials derived from the SPA impact.

How to cite: Andrews Hanna, J. C., Gowman, G., Wakita, S., Johnson, B. C., Alexander, A., Bill, C. A., Bottke, W. F., Broquet, A., Collins, G. S., Davison, T. M., Evans, A. J., Keane, J. T., Levin, J. N., Mallik, A., Marchi, S., Moriarty III, D. P., Moruzzi Fresenius, S. A., and Roy, A.: The South Pole-Aitken basin constrains the early evolution and differentiation of the Moon, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16091, https://doi.org/10.5194/egusphere-egu26-16091, 2026.

EGU26-16905 | ECS | Orals | PS7.2

Insights into pitted cones at Isidis Planitia through synthesis of interior and surface 

Jelte Bijlsma, Bart Root, and Sebastiaan de Vet

The Isidis Planitia impact basin on Mars is located on the north-south dichotomy boundary, bordered by Utopia Planitia and the Syrtis Major volcanic province. The basin records a long geological history of global and regional events of impact-induced, volcanic and sedimentary processes. This is evident in the presence of a high-density subsurface mass concentration, the strongest on Mars outside the major volcanic provinces. The nature of this interior structure remains poorly understood despite modelling efforts (e.g., [1-3]). Isidis Planitia’s surface also hosts the densest clustering of pitted cones [4,5]. The formation mechanism of these landforms, characterised by a conical mound with a central depression, remains debated as volcanic [6], sedimentary [4] or glacial [7].

We present an integrated approach to Isidis Planitia, showing that pitted cones are topographically constrained by surface wrinkle ridges driven by its subsurface structure. The subsurface is modelled using impact scaling laws combined with geological context to formulate a multi-layered model, which is fit to the local gravity field. Resultant structural elements are consistent with impact theory [8-10], estimated structures below Lunar basins [11,12], as well as mapped basins [13]. However, the gravity field cannot be constrained using infill, scaling laws and realistic density values. The models require mantle-like materials in the innermost parts of the basin. This element does not reconcile with expectations of impact theory nor basin infill, and is interpreted as significant post-impact plutonic intrusions.

This intrusive element is linked to a set of wrinkle ridge surface expressions with anomalous direction and dip. Two distinct formations of ridges are identified: an initial radial set of ridges and a latter concentric inward-dipping formation. This anomalous concentric set is not mirrored in Lunar basins [14,15] nor in Martian basins Utopia and Hellas [16,17]. The initial set is likely driven by regional compressive effects. The latter formation is driven by a stress field in the inner basin, which could be achieved during pluton inflation.

The pitted cones are shown to correlate with the basin topography dominated by the wrinkle ridges. The population conforms to both sets of pre-existing wrinkle ridges in distinct surface flow patterns. They are most consistent with volcanic rootless cones formed by lavas interacting with near-surface volatiles. The lava could be sourced from the intrusive magmatism, addressing the lack of other sources [6]. Overall, this study links Isidis Planitia’s subsurface structure to surface morphology. It could redefine the complex and dynamic basin, offering new insights into the active geological evolution of Mars.

References: [1] Wieczorek et al. (2022). [2] Ding et al. (2024). [3] Zhong et al. (2022). [4] Mills et al. (2024) Icarus 418. [5] Chen et al. (2024). [6] Ghent et al. (2012). [7] Guidat et al. (2015). [8] Freed et al. (2014). [9] Johnson et al. (2018). [10] Potter (2015). [11] Runyon et al. (2022). [12] Spudis et al. (2014). [13] Christeson et al. (2021). [14] Collins et al. (2023). [15] Tariq et al. (2024). [16] Carboni et al. (2025). [17] Head et al. (2002).

How to cite: Bijlsma, J., Root, B., and de Vet, S.: Insights into pitted cones at Isidis Planitia through synthesis of interior and surface, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16905, https://doi.org/10.5194/egusphere-egu26-16905, 2026.

EGU26-17615 | ECS | Posters on site | PS7.2

A Generalized Method for the three-dimensional characterization of the internal structure of planetary bodies based on Markov Chain Monte Carlo (MCMC) techniques 

Gabriele Boccacci, Martina Ciambellini, Anna Maria Gargiulo, and Antonio Genova

This study presents a novel Bayesian framework for the three-dimensional characterization of the internal structure of planetary bodies, accounting for their irregular layering. The interior model inversion is formulated within a Markov Chain Monte Carlo (MCMC) approach and relies on three-dimensional model equations linking the physical properties of the internal layers to the spherical harmonic coefficients of the gravity field. The method produces statistically consistent posterior distributions of parameters that define the internal structure of each accepted model that match the target distributions of the observed gravity coefficients and complementary geophysical constraints (e.g., Love number k2, librations).

Each interior model consists of concentric uniform ellipsoidal layers defined by size, density, and rheological properties. Crustal thickness variations are represented as deviations from a reference ellipsoid, providing a computationally efficient alternative to fully voxel-based representations while retaining sensitivity to lateral heterogeneities. Gravity coefficients are computed as the sum of a hydrostatic contribution, determined by the ellipsoidal shape of each layer, and a non-hydrostatic contribution derived from degree-dependent admittance.

The framework yields global grids of the crustal thickness together with the corresponding gravity spectra and associated residuals. These outputs provide constraints that cannot be captured by 1-D (spherical) or 2-D (ellipsoidal) interior models commonly adopted in the literature. The proposed approach is particularly suited to small bodies of the Solar System, including icy moons and dwarf planets, for which shape irregularities exert a first-order control on internal structure and geological evolution.

How to cite: Boccacci, G., Ciambellini, M., Gargiulo, A. M., and Genova, A.: A Generalized Method for the three-dimensional characterization of the internal structure of planetary bodies based on Markov Chain Monte Carlo (MCMC) techniques, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17615, https://doi.org/10.5194/egusphere-egu26-17615, 2026.

EGU26-19577 | ECS | Posters on site | PS7.2

Design and Performance of the MaCro Crosslink Radio Science Instrument for M-MATISSE 

Tobias Vorderobermeier, Tom Andert, Martin Pätzold, Silvia Tellmann, Dirk Plettemeier, Martin Laabs, Jan Budroweit, Takeshi Imamura, Hiroki Ando, Antonio Genova, Matthias Hahn, Katsuyuki Noguchi, Janusz Oschlisniok, Kerstin Peter, Wolfgang Schäfer, Beatriz Sanchez-Cano, and Francois Leblanc

The M-MATISSE mission, currently in Phase A with ESA as an M7 candidate, is a dual-spacecraft concept designed to investigate the coupled Martian magnetosphere, ionosphere, and thermosphere (MIT coupling) under varying space-weather and lower-atmosphere conditions. Two identical spacecraft, “Henri” and “Marguerite,” will fly complementary orbits with apocenters of 3,000 km and 10,000 km and common pericenters at 250 km, enabling highly diverse radio occultation geometries through an inter-satellite crosslink.

This contribution focuses on the M-MATISSE Crosslink Radio Science (MaCro) instrument, a dedicated mutual radio occultation payload optimized for Mars ionospheric and atmospheric profiling. MaCro employs software-defined radios based on the AD9361 transceiver, dual-band omnidirectional antenna assemblies (UHF/S-band), and ultrastable master reference oscillators with Allan deviation on the order of 10⁻¹³ at 100 s. Simultaneous UHF and S-band links allow separation of dispersive ionospheric effects from neutral atmospheric contributions, while flexible SDR filtering and automatic gain control accommodate large signal dynamics during occultation ingress and egress.

We present the MaCro instrument architecture and its expected performance, highlighting design challenges specific to crosslink radio occultation instruments. We provide bounds on the achievable frequency and refractivity retrieval accuracy and its sensitivity to the carrier-to-noise ratio, integration time, and clock stability, and discuss the implications for high-resolution profiling of Mars’ ionosphere and neutral atmosphere.

How to cite: Vorderobermeier, T., Andert, T., Pätzold, M., Tellmann, S., Plettemeier, D., Laabs, M., Budroweit, J., Imamura, T., Ando, H., Genova, A., Hahn, M., Noguchi, K., Oschlisniok, J., Peter, K., Schäfer, W., Sanchez-Cano, B., and Leblanc, F.: Design and Performance of the MaCro Crosslink Radio Science Instrument for M-MATISSE, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19577, https://doi.org/10.5194/egusphere-egu26-19577, 2026.

EGU26-21183 | Posters on site | PS7.2

Uranus gravity field investigations from an orbiter mission 

Daniele Durante and Ivan di Stefano

High-precision radio tracking from a future Uranus orbiter may provide key constraints on Uranus’ internal structure and dynamics, provided suitable instrumentation and an optimized orbital tour. We present the results of radio science simulations to evaluate gravity field recovery performance across different orbital configurations.

We run numerical simulations of the gravity experiment by using NASA/JPL MONTE orbit determination software, assuming the orbiter to be equipped with high-end radio tracking system capable of generating accurate Doppler and range observables at both X- and Ka-band, supporting triple-link plasma calibration. Two representative mission scenarios are analyzed: (i) southern-hemisphere periapses at an altitude of ~7000 km, passing outside the ring system, and (ii) low-altitude periapses at ~1000 km, passing inside the rings. The results show indeed a strong dependence of gravity field recovery on orbital geometry. In the higher-altitude scenario, only the J2 and J4 zonal harmonics can be estimated with sufficient accuracy, whereas the lower-altitude configuration enables the reliable determination of J6.

In parallel, we investigate the effect of Uranus’ normal modes of oscillation on the spacecraft dynamics. The free oscillation spectrum is computed assuming a simplified internal structure model, adapted from approaches developed for the Juno and Cassini missions. Although individual mode frequencies are unlikely to be resolved, their cumulative effect produces time-variable perturbations on the low-degree zonal harmonics that may act as a source of noise in gravity field estimation.

These results highlight the critical role of high-end radio tracking instrumentation and orbital design in maximizing the scientific return of gravity science at Uranus and provide a quantitative framework for evaluating the observability of its interior and dynamical processes.

How to cite: Durante, D. and di Stefano, I.: Uranus gravity field investigations from an orbiter mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21183, https://doi.org/10.5194/egusphere-egu26-21183, 2026.

EGU26-22989 | ECS | Posters on site | PS7.2

Integration of Radio Tracking and Feature-based Optical Measurements for Geophysical Investigations 

Anna Maria Gargiulo, Simone Andolfo, Tommaso Torrini, Cristina Re, and Gabriele Cremonese

Accurate estimation of geophysical parameters, including total mass, moment of inertia and rotational state of planetary bodies is essential for understanding their degree of differentiation, constraining their internal structure, and gaining insights into their evolutionary path. To improve the accuracy of these key estimates, we have developed an integrated framework that combines Earth-based radio tracking data with navigation measurements based on the observation of relevant surface features on the body’s surface.

Two-way Doppler and range measurements provide robust constraints on the spacecraft motion along the line of sight and are traditionally used for gravity and geophysical investigations. Surface imagery of the central body offers complementary information, supporting the estimation of the target body’s spin vector and deviations from uniform rotational state, such as longitudinal librations.

The proposed approach leverages the tracking of relevant surface features to jointly reconstruct the spacecraft trajectory and estimate geophysical parameters of the target body. Features tracked across partially overlapping images acquired sequentially during closely spaced orbital passes improve the internal consistency of the trajectory reconstruction, whereas features observed across different mission phases contribute to the refinement of the body’s rotational state. To address challenges arising from variable illumination conditions and resolution discrepancies in planetary images, hybrid strategies are adopted for feature tracking, combining conventional computer vision with Artificial Intelligence-based feature detection and matching.

The framework is validated using data from the MESSENGER spacecraft during its science orbital phase around Mercury. The novel approach improves estimation accuracies with respect to single-instrument solutions and provides a flexible, effective tool for maximizing the scientific return of deep-space missions.  

How to cite: Gargiulo, A. M., Andolfo, S., Torrini, T., Re, C., and Cremonese, G.: Integration of Radio Tracking and Feature-based Optical Measurements for Geophysical Investigations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22989, https://doi.org/10.5194/egusphere-egu26-22989, 2026.

EGU26-23097 | ECS | Posters on site | PS7.2

Structural Controls on Volcanic Eruptions: Insights from the Copland-Rachmaninoff Tectonic Regime on Mercury 

Gene Schmidt, Salvatore Buoninfante, Valentina Galluzzi, and Pasquale Palumbo

Tectonic activity from global contraction and its influence on the location of volcanic eruptions (i.e. faculae) continues to elicit diverse interpretations, with the underlying structural controls of many faculae still poorly constrained [1;2]. At the boundary of the Rachmaninoff basin area and the northern smooth plains lies a large 800 km long, 100km wide, and 1000-3500 km high elevation structure which terminates at the 200 km diameter Copland crater. 400 km north of this boundary is a parallel structure of similar dimensions, implying a shared formation mechanism. Topographic profiles perpendicular to these structures reveal that both have asymmetric positive relief indicative of thrust fault scarps (i.e. lobate scarps and rupes), with a steep sloping forelimb followed by a more gently sloping backlimb. Although these structures are generally taller and wider than even the largest thrust fault scarps on Mercury (e.g. Enterprise Rupes with <2500 m of relief), we present evidence that these structures contain a significant amount of shortening and may be unidentified thrust faults which strike east and dip to the south. Specifically, they outline the rims of relic craters (b50 and b72, [3]), meaning that crustal shortening utilized preexisting crater wall bounding normal faults. This shortening is identified from the deformation induced on Copland crater where its southern rim is elevated 1,250 m respect to its northern rim. Mapped faults in the area have noted smaller lobate scarps in the area, and one which passes through the center of Copland and offsets its floor by 400 m [4], however this is dwarfed by the deformation caused by the deflected large thrust which has uplifted the southern rim of Copland crater. Furthermore, the presence of volcanic eruptions (Neidr and Nathair Faculae, [5]) along the southern edge of the scarp, the hanging wall, is typical of thrust fault activity on Earth [6]. The parallel trend shared with the long-wavelength topography (broad troughs and crests, [7]) may also indicate a shared formation mechanism. Revelations from the BepiColombo mission, particularly the updated high-resolution topography, will facilitate more interpretation of the local tectonic regimes on Mercury and may reveal many undetected shortening structures and faculae, and in turn a full appreciation of their geospatial relationships can be achieved.

References

[1] Banks, M. E. et al. (2015). JGR: Planets, 120(11), DOI: 10.1002/2015JE004828

[2] Jozwiak, L. M., et al. (2018). Icarus, 302, 191-212. DOI: 10.1016/j.icarus.2017.11.011

[3] Orgel, C., et al. (2020). JGR: Planets, 125(8), e2019JE006212. DOI: 10.1029/2019JE006212

[4] Bernhardt, H., et al. (2025). (No. EPSC-DPS2025-2108). Copernicus Meetings. DOI: 10.5194/epsc-dps2025-2108

[5] Wright, J., et al. (2024). Earth and Space Sci., 11(2). DOI: 10.1029/2023EA003258

[6] Gaffney, E. S., et al. (2007). Earth and Planet. Sci. Let., 263(3-4), 323-338. DOI: 10.1016/j.epsl.2007.09.00

[7] Schmidt, G. W., et al. (2026). JGR: Planets, 120(11). DOI: 10.1029/2025JE009233

Acknowledgements: We gratefully acknowledge funding from the Italian Space Agency (ASI) under ASI-INAF agreement 2024-18-HH.0.

How to cite: Schmidt, G., Buoninfante, S., Galluzzi, V., and Palumbo, P.: Structural Controls on Volcanic Eruptions: Insights from the Copland-Rachmaninoff Tectonic Regime on Mercury, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23097, https://doi.org/10.5194/egusphere-egu26-23097, 2026.

 

The Boulby Underground Laboratory (BUL) is the UK’s deep underground science facility located in north-east of England, 1.1 km below the surface in the ICL Boulby Mine, an active polyhalite mine.  

BUL was established in 1988 to search for dark matter, because with an overburden of 2805 meters water equivalent, the cosmic radiation is decreased a million-fold, making BUL one of a few underground laboratories around the world suitable for experiments requiring low background radiation conditions. In the beginning, BUL was purely focused on rare-event searches but has since branched out into multidisciplinary studies and the establishment of a biosciences programme.  

The current underground facility includes clean room laboratory space and an Outside Experimentation Area, as well as expansion plans for an underground laboratory five times the size of the current one. The Outside Experimentation Area is well-suited for astrobiology research and analogue space studies, as it is in a layer of 200-million-year-old salt, in a hot, dusty and, in a sense, extreme environment. The flagship of the bioscience programme is the Mine Analogue Research (MINAR) Programme which BUL has hosted since 2013 in collaboration with the University of Edinburgh UK Centre for Astrobiology. Arranged yearly, MINAR brings together international teams from NASA, ESA, and universities in the UK and abroad down to Boulby for a short duration to study life in the extreme and test planetary exploration technologies. 

We will give a summary of the Boulby underground laboratory and environment, and the past, present and future of our biosciences programme, with special attention to its role as an analogue site for space exploration. The Boulby lab is funded and operated by the Science and Technologies Facilities Council (STFC) operating under the United Kingdom Research and Innovation. 

How to cite: Puputti, J.: Biosciences at Boulby Underground Laboratory: a Deep Subsurface Analogue Test Environment for Planetary Exploration and Astrobiology , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-111, https://doi.org/10.5194/egusphere-egu26-111, 2026.

EGU26-2594 | Posters on site | PS7.3

Landslides and nearby impact events on Ceres: evidence of triggering through morphological analysis and absolute model dating 

Maria Teresa Brunetti, Marco Emanuele Discenza, Lisa Molaro, Mariacarmela Minnillo, Goro Komatsu, and Enrico Miccadei

Landslides are widespread geomorphic features on solid bodies across the Solar System [1]. On Ceres, a densely cratered dwarf planet, landslides are common [2-5] and affect more than 20% of craters larger than 10 km [4]. However, their triggering mechanisms remain poorly constrained given the absence of active geological processes. Previous studies have proposed two impact-related landslide triggers on Solar System bodies: i) direct strikes on pre-existing slopes [4] and, ii) impact-induced ground shaking [6,7].

Based on criteria including freshness, well-defined margins, optimal illumination and no crater saturation, we selected eight landslides  ̶ out of fifty-seven associated with nearby impact craters  ̶  for detailed morphological analysis. All of the selected landslides occurred on the outer rim of impact craters, and in most cases within the wall of an older, pre-existing crater. Each landslide was mapped using high-resolution LAMO imagery and the 100 m global shape model [8].

Crater size-frequency distributions were measured on both landslide deposits and impact crater ejecta using two approaches: i) including all craters and, ii) considering only primary craters. A Voronoï tessellation was used to filter out secondary impact areas [9], and absolute model ages were computed using the lunar-derived model [10].

The crater counting method revealed that the eight landslides are geologically young, ranging from ~13.5 Ma to ~107 Ma. Notably, these ages are consistent with those of the nearby impact crater ejecta, indicating a temporal overlap between landslides and impact events.

Overall, the analyses revealed a spatial and temporal correlation between the landslides and nearby impacts on Ceres, which provides evidence for the mechanism that triggered the mass movements [12]. The results from Ceres show that this approach is effective in identifying similar relationships between impact events and landslides on other Solar System bodies.

 

References:

[1] Brunetti M. T. and S. Peruccacci (2023) Oxford Res. Encyclop. Planet. Sci.

[2] Schmidt B. E. et al. (2017) Nature Geosci. 10, 338–343

[3] Chilton H. T. et al. (2019) J. Geophys. Res. Planets 124, 1512–1524

[4] Duarte K. D. et al. (2019) J. Geophys. Res. Planets 124, 3329–3343

[5] Parekh, R. et al. (2021) J. Geophys. Res. Planets 126, e2020JE006573

[6] Neuffer D. P. and R. A. Schultz (2006) Q. J. Eng. Geol. Hydrogeol. 39, 227–240

[7] Bickel V. T. et al. (2020) Nat. Commun. 11, 2862

[8] Park R. S. et al. (2019) Icarus 319, 812–827

[9] Discenza et al. (2022) Planet. Space Sci. 217, 105503

[10] Hiesinger et al. (2016) Science 353, 6303

[11] Discenza et al. (2025) Commun. Earth & Environ. 6, 1042

How to cite: Brunetti, M. T., Discenza, M. E., Molaro, L., Minnillo, M., Komatsu, G., and Miccadei, E.: Landslides and nearby impact events on Ceres: evidence of triggering through morphological analysis and absolute model dating, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2594, https://doi.org/10.5194/egusphere-egu26-2594, 2026.

EGU26-6966 | ECS | Posters on site | PS7.3

Monte Carlo simulations of the Martian surface and subsurface radiation environment for human missions 

Nicole Orientale, Lorenzo Bonechi, Diletta Borselli, Raffaello D'Alessandro, Catalin Frosin, and Sandro Gonzi

One of the most critical challenges to expand human exploration on the surface of Mars is radiation protection for astronauts on long-duration missions, due to the severe health effects that can be caused by long-term exposure to radiation.

In space there are two main sources of radiation: Galactic Cosmic Rays (GCRs) and Solar Particle Events (SPEs). Mars does not have an intrinsic magnetic field capable of providing any significant shielding from space radiation. As a result, energetic particles in GCRs and SEPs can penetrate the Mars atmosphere and interact with the atmosphere, before reaching the surface, and with the Martian subsurface, generating many secondary particles. These interactions result in a complex radiation spectrum, given by primary and secondary particles, that depend on the planetary atmospheric and geological properties. An understanding of the Martian radiation environment is important to identify potential natural shelters for astronauts, that can lead to incoming radiation loss of energy through ionization processes and provide a long-term reduction of the exposure to radiation from above. Possible shelter candidates are subterranean lava tubes, natural underground tunnels formed by flowing lava that cools and solidifies on the surface while molten lava continues to flow beneath, that can be large and structurally stable, potentially offering natural protection from cosmic radiation, solar wind, strong temperature excursion, dust and micrometeorite impacts, for future exploration and habitation. Recent works [1] have highlighted the presence on Mars of voluminous underground caves and potential lava tubes with sizes typically ranging from around 50 meters and depths often exceeding 100 meters.

We implemented Monte Carlo simulations, using CORSIKA 8 [2] [3] and FLUKA [4], to study the radiation environment on Mars, with a precise modelling of the cascade of secondary particles generated during interactions and a detailed atmospheric model. Therefore, we made a precise quantification of the change of particle spectra under different shielding environment like at Martian surface, subsurface and within Martian caves, for different given subsurface compositions and solar activity conditions. Also, we compared the simulated radiation levels within caves to surface conditions, in order to quantify the benefits offered by subsurface environments.

[1]           Sauro F., et al., Lava tubes on Earth, Moon and Mars: A review on their size and morphology revealed by comparative planetology, Earth Science  Reviews, 2020.

[2]           Engel R., et al., Towards A Next Generation of CORSIKA: A Framework for the Simulation of Particle Cascades in Astroparticle Physics, 2019.

[3]           Alameddine J. M., et al., Simulating radio emission from particle cascades with CORSIKA 8, 2025.

[4]           Battistoni G., et al., Overview of the FLUKA code, Annals of Nuclear Energy, 2015.

How to cite: Orientale, N., Bonechi, L., Borselli, D., D'Alessandro, R., Frosin, C., and Gonzi, S.: Monte Carlo simulations of the Martian surface and subsurface radiation environment for human missions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6966, https://doi.org/10.5194/egusphere-egu26-6966, 2026.

EGU26-10438 | ECS | Posters on site | PS7.3

Designing a penetrating radar system for lunar surveys as part of the HARLOCK project 

Giuseppe Esposito, Gianluca Gennarelli, Carlo Noviello, Giovanni Ludeno, Ilaria Catapano, and Francesco Soldovieri

Developing science-driven instrumentation and methodologies for the investigation of lunar subsurface materials, such as water ice, and surface to near-surface mineral resources is the main goal of HARLOCK (High-resolution Autonomous Resource Lunar Observation & Characterization Kit) project, which is a strategic Italian project coordinated by CNR and INAF, as part of the PRORIS initiative [1].

Among the HARLOCK technologies, the penetrating radar is one of the few ones having a high Technology Readiness Level since it has been an effective payload for rover and lander adopted in Moon observation missions, for instance the China missions Chang'e-3-6 [2] - [6]. However, as well-known, the penetrating radar provides a high-resolution subsoil image only once the collected data are processed properly. In this frame, an open issue is the design of imaging approaches based on reliable mathematical models of signal propagation and diffraction in stratified media (air/soil), whose electromagnetic characteristics are typical of the planetary environment of interest. Furthermore, another relevant issue is the capability of exploiting the increased information content offered by multi-antenna systems collecting data by using more than one transmitting and receiving antenna.

This contribution deals with two imaging approaches for multi-antenna penetrating radar systems, which face the imaging in a stratified medium as a linear inverse scattering problem. The approaches exploit two different ray-based propagation models: Interface Reflection Point (IRP) model and  Equivalent Permittivity (EP) model. These models were previously proposed for single transmitter single receiver penetrating radar system [7], and adopted to process Chang'E-4 Lunar Penetrating Radar data [8]. Specifically, a performance analysis comparing the approaches in terms of reconstruction capabilities and computational burden will be presented at the conference. It is worth pointing out that the performance analysis in terms of resolution supports the definition of the penetrating radar system requirements for a given soil, while considering the size of the objects to be detected. Furthermore, computational efficiency is essential to move towards real time imaging.

References

[1] PRORIS Consortium (2024), PRORIS – Programma di Ricerca Spaziale di Base, INAF–CNR Joint Program. Available at: https://www.proris.it

[2] Ip, W.-H., et al. Preface: The Chang’e-3 lander and rover mission to the Moon. Res. Astron. Astrophys. 14, 1511, 2014.

[3] Jia, Y. et al. The scientific objectives and payloads of Chang’E− 4 mission. Planet. Space Sci. 162, 207–215, 2018.

[4] Li, C. et al. The Moon's farside shallow subsurface structure unveiled by Chang'E-4 Lunar Penetrating Radar, Science Advances, 6 (9), 2020.

[5] Su, Y. et al. Hyperfine Structure of Regolith Unveiled by Chang’E-5 Lunar Regolith Penetrating Radar. IEEE Trans. Geosci. Remote Sens. 60, 1–14 (2022)

[6] Li, C. et al. Nature of the lunar farside samples returned by the Chang’E-6 mission. Natl. Sci. Rev. nwae328, 2024.

[7] Catapano, I. et al. Contactless ground penetrating radar imaging: State of the art, challenges, and microwave tomogra-phy-based data processing. IEEE Geoscience and Remote Sensing Magazine, 10.1: 251-273, 2021.

[8] Soldovieri, F. et al. Microwave tomography for Lunar Penetrating Radar data processing in Chang'e 4 mission. Scientific Reports, 15(1):5219, 2025.

How to cite: Esposito, G., Gennarelli, G., Noviello, C., Ludeno, G., Catapano, I., and Soldovieri, F.: Designing a penetrating radar system for lunar surveys as part of the HARLOCK project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10438, https://doi.org/10.5194/egusphere-egu26-10438, 2026.

EGU26-12311 | ECS | Posters on site | PS7.3

Martian Surface / Atmosphere Web Interface 

Fabio Massimo Grasso, Simone Silvestro, Umberto Rizza, David Alegre Vaz, and Lori Fenton

Aeolian processes are a dominant agent of surface modification on Mars, and the distribution, orientation, and morphology of wind-formed bedforms provide key constraints on both present-day atmospheric circulation and past climatic conditions. However, direct measurements of near-surface winds are limited to a small number of landing sites, restricting our ability to characterize wind regimes at regional and global scales. Atmospheric General Circulation Models (GCMs) therefore play a central role in reconstructing Martian wind patterns, but their outputs require substantial post-processing to be meaningfully compared with geomorphological observations. Systematic and accessible tools that link atmospheric simulations to aeolian surface processes are essential for model validation and for interpreting the climatic significance of observed landforms.
We present the Martian Surface/Atmosphere Web Interface, a freely accessible, web-based platform designed to facilitate the investigation of wind-driven sediment transport and bedform formation on Mars. The interface is built upon atmospheric simulations produced by the NASA Ames Global Circulation Model and provides an integrated workflow that converts modeled near-surface winds into quantitative predictions of sand flux and bedform orientations. By enabling remote execution of computationally intensive analyses through a user-friendly interface, the platform removes the need for local installations and specialized expertise in handling large GCM datasets.
Sand fluxes are derived using two complementary parameterizations that reflect different physical assumptions about aeolian transport. The first follows the formulation of Kok (2010), which accounts for saltation hysteresis by distinguishing between fluid and impact thresholds, allowing sediment transport to persist under lower wind stresses. The second approach is based on Rubanenko et al. (2023) and adopts the Martin and Kok (2017) saltation flux law, which assumes a linear scaling of sediment flux with shear stress, supported by field observations and theoretical considerations of splash-dominated entrainment. The parallel implementation of these formulations allows users to evaluate the sensitivity and robustness of transport predictions.
The resulting sand fluxes are further used to estimate bedform orientations through implementations of two end-member formation mechanisms: the bed instability mode and the elongation mode. The interface provides directional statistics and circular plots of transport vectors, enabling rapid comparison between modeled wind regimes and observed aeolian patterns. The underlying simulation dataset spans approximately the last 400 kyr of Martian climate history and explores a broad range of climatic scenarios, including variations in atmospheric pressure, axial obliquity, orbital eccentricity, and longitude of perihelion. These parameters capture the influence of orbital forcing and atmospheric density on near-surface winds and sediment transport.
The Martian Surface/Atmosphere Web Interface provides a unified and accessible framework to explore surface–atmosphere interactions across Mars. It supports the validation of atmospheric models, aids in distinguishing active from relict aeolian landforms, and offers new opportunities to investigate the role of climatic variability in shaping the Martian surface through time.

How to cite: Grasso, F. M., Silvestro, S., Rizza, U., Vaz, D. A., and Fenton, L.: Martian Surface / Atmosphere Web Interface, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12311, https://doi.org/10.5194/egusphere-egu26-12311, 2026.

EGU26-19426 | Posters on site | PS7.3

Identifying and Protecting Geological Heritage in the Solar System 

Barbara De Toffoli

The pace of space exploration has visibly accelerated, reminiscent of the 1960s space race era. However, following this reinvigorated drive to establish a presence in the Solar System, a critical issue demands attention: exogeoconservation, the protection of irreplaceable geological heritage on celestial bodies beyond Earth. As scientific and commercial ventures prepare to exploit extraterrestrial resources at increasingly faster pace, exogeoconservation can no longer be ignored. The worlds we seek to explore and exploit contain invaluable records of Solar System evolution and quantitative, data-driven foundations are now required for balanced policies enabling responsible resource utilization while protecting the geological heritage.

While planetary protection policies set strict rules to prevent biological contamination of other worlds, no parallel system exists for managing the impact on abiotic environments and materials. Over 20 years ago, the concept of "planetary parks" was proposed to protect unique geological sites [1]. More recently, authors have called for the establishment of exogeoconservation as a discipline based on terrestrial geoconservation practices that protect geoheritage, i.e. geological features of scientific, cultural or aesthetic importance [2]. However, implementation has stalled.

Existing international laws like the Outer Space Treaty lack mechanisms to identify and designate geological conservation areas on celestial bodies. And, although it has been proposed to draw an example from the Antarctic Treaty System’s regulation system, a fundamental barrier remains: criteria for identifying exogeoheritage features are undefined and attempts to directly translate geoconservation methods to Mars using orbital data have failed to pinpoint targets for protection [3]. This underscores the fundamental lack of strategies and policies to inventory and assess the significance of extraterrestrial geological environments in the context of a fast evolving exploration pace. On Earth, geoconservation relies on extensive field mapping and hierarchization based on rarity, scientific value, and other factors, and now analogous exogeoheritage assessment tools and benchmarks tailored to remote planetary data are needed. The new space race era presents both challenges and opportunities, and it is a collective responsibility to seize this moment and chart a course that balances progress with conservation.

 

[1] Cockell, C., & Horneck, G. (2004). A planetary park system for Mars. Space policy, 20(4), 291-295.

[2] Matthews, J. J., & McMahon, S. (2018). Exogeoconservation: Protecting geological heritage on celestial bodies. Acta Astronautica, 149, 55-60.

[3] Fletcher, C., Van Kranendonk, M., & Oliver, C. (2025). Practical exogeoconservation of Mars: Lessons from the Mars Desert Research Station, Utah. Planetary and Space Science, 256, 106038.

How to cite: De Toffoli, B.: Identifying and Protecting Geological Heritage in the Solar System, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19426, https://doi.org/10.5194/egusphere-egu26-19426, 2026.

The “Earth Moon Mars” (EMM) Research Infrastructure has been established within the framework of the Italian National Recovery and Resilience Plan (PNRR) to support scientific activities across multiple domains, particularly in the areas of Planetary Sciences and Earth Observation. EMM is conceived as a distributed research ecosystem articulated into a set of complementary elements, including an upgrade of the Sardinia Radio Telescope aimed at extending its reception capabilities to deep-space signals, an initiative addressing feasibility studies and prototypical developments for a lunar outpost and Moon-based instrumentation for Universe and Earth observation, and the Earth and Mars Research Network (EMN), which provides an integrated system specifically designed to enable long-term observational, modelling, and data integration capabilities across Earth and planetary science domains. EMM is the outcome of a joint effort involving the National Institute for Astrophysics (INAF), the National Research Council (CNR), and the Italian Space Agency (ASI), which contribute distinct but synergistic expertise and assets.

At the time of writing, the EMM Research Infrastructure is evolving from an initial construction and consolidation phase toward a fully operational configuration. Within this context, the present contribution focuses on the EMN component, realized as  a composite and distributed system that implements an end-to-end scientific workflow, ranging from observations to modelling activities. EMN integrates heterogeneous elements including hardware facilities, software environments, data resources, and consolidated scientific and technological know-how. Its architecture supports the full observational and analytical chain, encompassing calibration and validation of satellite data, radiative transfer modelling, data fusion approaches, data assimilation systems, and meteorological and climate models applicable to both terrestrial and planetary atmospheres.

A central aspect of EMN lies in its capacity to promote interaction and cross-fertilization between Earth Observation and Planetary Sciences communities. This interaction is pursued through the integration of observational assets and modelling tools, as well as through the harmonization of methodologies and workflows that are traditionally developed within separate disciplinary contexts. In this sense, EMN provides a structure in which observational data and modelling activities are jointly exploited, enabling consistent interpretation and enhanced scientific use of multi-source datasets.

The contribution outlines how the various EMN segments have been progressively developed during the course of the EMM project These include observational infrastructures, modelling and simulation environments, data processing and analysis chains, and knowledge-based components supporting interpretation and scientific exploitation. Together, these elements form an integrated system designed to operate across a wide range of spatial and temporal scales.
EMN is expected to enter its operational phase in 2026 and will be made available to the international scientific community for at least a decade, supporting a wide range of Earth and planetary science applications. While operating as an autonomous component, EMN remains tightly integrated with the other elements of the EMM Research Infrastructure, contributing to its overall coherence and long-term sustainability.

How to cite: Cortesi, U.: The Earth and Mars Research Network: an end-to-end component of the EARTH MOON MARS Research Infrastructure , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21448, https://doi.org/10.5194/egusphere-egu26-21448, 2026.

EGU26-21837 | Posters on site | PS7.3 | Highlight

Human Factors in Lunar Boulder Mapping: Can Citizen Scientists Support Experts? 

Sandro Rossato, Laura Criscuolo, Cristina Da Lio, Gregorio Dal Sasso, Gianluca Frasca, Valentina Marzia Rossi, Gianna Vivaldo, Luca Zaggia, Maurizio Pajola, and Filippo Tusberti

While AI and neural networks automation advance, human interpretation of planetary imagery remains essential for mapping surface features, yet it introduces uncertainty due to variable expertise, fatigue, and ambiguous boundaries. Standardized protocols, best practices, and scalable participation are increasingly important to ensure reproducibility while addressing the growing volume of data. This study examines whether non‑expert individuals, after targeted training, can integrate with or substitute expert researchers in identifying and mapping boulders on the lunar surface, and quantifies where human variability most affects outcomes.

Two high‑resolution Lunar Reconnaissance Orbiter image subsets in Mare Crisium, east of the Luna‑24 landing site and adjacent to a fresh ~1‑km Copernican crater, served as test areas (pixel scale ~0.5 m). An expert benchmark was established by three professional mappers and compared against two participant cohorts: 26 trainees from a winter school focused on planetary geological mapping and 65 amateur astronomers contributing via Zooniverse, a Citizen‑Science web platform. All participants received concise training to independently map two areas with different boulder densities. Detection performance and internal consistency were evaluated as a function of observer-related factors, image features, and boulder size/density, alongside the impact of simple workflow rules designed to reduce ambiguity.

Results reveal observer‑dependent variability, with larger discrepancies in the amateur cohort, particularly in dense fields and for smaller features close to the detection threshold. Agreement is highest on isolated, high‑contrast boulders and declines where shadowing, albedo variations, or overlapping features complicate the interpretation. Short, standardized criteria and targeted examples reduce differences in results between observers, especially among trainees, while improving repeatability within each cohort. Aggregating multiple non‑expert annotations and applying basic quality gates, such as mapped features abundance, produces outputs approaching expert‑level reliability.

Non‑expert contributors, when provided with focused instruction and lightweight quality control, can reliably augment expert efforts in lunar boulder mapping, particularly for routine counting and mapping in simple settings. However, they do not fully substitute experts in ambiguous contexts, where professional judgment remains remarkably better for consistent classification and boundary decisions. These findings support an hybrid approach combining expert‑defined standards, brief training modules, consensus‑based citizen contributions, and standardized workflows to enhance throughput without compromising scientific robustness, reliability, and consistency. More broadly, the structured approach demonstrated here, by combining expert-defined standards, targeted training, and consensus mechanisms, offers a potentially transferable methodological framework for research domains facing similar challenges of graphic data volume and interpretive complexity.

How to cite: Rossato, S., Criscuolo, L., Da Lio, C., Dal Sasso, G., Frasca, G., Rossi, V. M., Vivaldo, G., Zaggia, L., Pajola, M., and Tusberti, F.: Human Factors in Lunar Boulder Mapping: Can Citizen Scientists Support Experts?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21837, https://doi.org/10.5194/egusphere-egu26-21837, 2026.

EGU26-21972 | Posters on site | PS7.3

Prokaryotic Communities in polar Brines: Ecological and Astrobiological Insights from Antarctica 

Maurizio Azzaro, Angelina Lo Giudice, Alessandro Ciro Rappazzo, Mauro Guglielmin, and Maria Papale

Brine pockets embedded within Antarctic permafrost and subglacial environments represent natural laboratories for studying microbial life under polyextreme conditions—high salinity, sub-zero temperatures, and oligotrophy. These analogues to extraterrestrial environments, such as the sub-ice oceans of Europa or the briny regolith of Mars, are crucial to astrobiological investigations looking to define the limits of life. As part of the Italian National Research Programme in Antarctica (PNRA) in the framework of the CLICPERECO project, a structured sampling campaign was conducted in the Tarn Flat (TF) area of Northern Victoria Land, where multiple brine inclusions were discovered and sampled. Samples were collected from a triangular sampling grid with vertices TF1, TF2, and TFB, each 18 meters apart, and from a central point (TF3) at three depths: 380, 460, and 510 cm (TF3-380, TF3-460, TF3-510), along with a sediment sample at the lake bottom (SED-TF3). DNA was extracted using the DNeasy PowerSoil Kit, followed by 16S rRNA gene amplicon sequencing on the Illumina HiSeqX platform. Taxonomic assignment was performed using the SILVA 138.1 database. The prokaryotic community displayed substantial spatial and vertical heterogeneity. Across all samples, Actinomycetota, Bacteroidota, and Proteobacteria were the dominant phyla. In the triangular grid, Actinomycetota reached over 32% at TF1 and TFB, while Cyanobacteriota dominated TF2 (29.4%), suggesting influence from light exposure or surface dynamics. In the central borehole, clear depth-related stratification was observed. Actinomycetota decreased from 48.9% at TF3-380 to 14.6% at TF3-510, whereas anaerobic lineages like Thermodesulfobacteriota (from 0.02% to 4.3%) and Campylobacterota (up to 2.1%) increased with depth, indicating a shift toward more reduced conditions. At the genus level, “Candidatus Aquiluna” and Ilumatobacter dominated surface layers, while deep samples harbored sulfate reducers such as Desulfoconvexum, Desulfuromusa, and Geopsychrobacter. The genus Thiomicrorhabdus surged from <0.01% in surface layers to >11.6% at 460 cm, further indicating sulfur-driven metabolisms in deeper brines. The detection of high abundances of Patescibacteria (up to 7.5% at TF3-460), a superphylum comprising ultra-small, often symbiotic bacteria, suggests that deep brine ecosystems may support complex, syntrophic microbial interactions.

These findings highlight the presence of stratified, diverse microbial consortia finely tuned to microenvironmental gradients within analysed brines. The ecological novelty and functional potential of these communities extend the known boundaries of microbial life on Earth and offer compelling analogies for life detection strategies beyond our planet. Future work integrating metagenomics, metabolomics, and in situ geochemical measurements will be crucial to uncover the evolutionary and adaptive mechanisms underlying life in these cryo-habitats.

How to cite: Azzaro, M., Lo Giudice, A., Rappazzo, A. C., Guglielmin, M., and Papale, M.: Prokaryotic Communities in polar Brines: Ecological and Astrobiological Insights from Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21972, https://doi.org/10.5194/egusphere-egu26-21972, 2026.

EGU26-620 | ECS | Posters on site | PS1.4

Thermal moonquakes at the lunar south pole: New evidence from Chandrayaan-3 ILSA observations 

Arghya Kusum Dey, Rahul Biswas, Kusham Sandhu, and Prakash Kumar

Thermal moonquakes are a series of repetitive seismic signals exhibiting nearly identical waveform patterns and amplitudes that occur periodically with the lunar diurnal cycle. India’s Chandrayaan-3 mission, which successfully landed in the south polar region of the Moon, deployed the Instrument for Lunar Seismic Activity (ILSA) to record ground accelerations at the landing site (69.37°S, 32.32°E) between August 24, 2023, and September 4, 2024. The instrument also monitored local surface temperatures, revealing extreme variations ranging from –20 °C to +60 °C.

After preliminary data processing, distinct thermal moonquakes were identified. The objective of this study is to analyze their frequency-dependent characteristics and investigate temperature-driven signatures. Based on waveform morphology, the thermal moonquakes are classified into three types: impulsive, intermediate, and emergent. Among these, emergent events are natural and occur due to the extension and contraction of lunar rocks, whereas the impulsive and intermediate events are caused by rover movement and other experiments conducted during the mission.

An additional focus of this research is to estimate the source locations of the thermal moonquakes using a chi-squared iterative single-station event-location algorithm. Assuming that seismic energy propagates along a one-dimensional path through a near-surface velocity model, we perform a grid search over latitude and longitude to identify the most probable source regions. Our results suggest that natural thermal moonquakes may originate from thermally induced stresses caused by large diurnal temperature variations in the lunar regolith, which reduce rock elasticity and lead to cracking and micro-fracturing.

The lunar south polar region remains one of the most intriguing yet least explored areas on the Moon. This study provides new insights into its near-surface mechanical behavior, offering a significant contribution toward understanding thermal stress-induced seismicity and the geophysical environment of the lunar south pole.

Keywords: Thermal moonquakes; Chandrayaan-3; ILSA; Lunar south pole; Thermal stress-induced seismicity; Single-station event location; Lunar regolith; Diurnal temperature variation.

How to cite: Dey, A. K., Biswas, R., Sandhu, K., and Kumar, P.: Thermal moonquakes at the lunar south pole: New evidence from Chandrayaan-3 ILSA observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-620, https://doi.org/10.5194/egusphere-egu26-620, 2026.

EGU26-630 | ECS | Posters on site | PS1.4

Stable Sr Variations in Impactites of Lonar Impact Crater, India: A Terrestrial Analogue for Lunar Crustal Evolution  

Gaurav Singh Papola and Ramananda Chakrabarti

Impact craters are ubiquitous features on surfaces of planetary bodies in the inner Solar System. Impact cratering exposes subsurface materials, making them valuable for studying subsurface compositions of planetary bodies. The ~1.88 km diameter Lonar crater in India is a simple crater that formed by the impact of a chondritic impactor ~570 ka ago [1,2]. This is a well-preserved crater hosted entirely within the ~66 My old Deccan continental flood basalts, making it an ideal terrestrial analogue for craters on the basaltic surfaces of other planetary bodies like the Moon. We report geochemical and stable (δ88Sr) and radiogenic (87Sr/86Sr) Sr isotopic compositions of six target basalts and nine impact melt breccias sampled from the upper crater wall and the distal ejecta blanket [2,3]. Geochemical measurements were performed using an ICP-MS (Thermo Scientific iCAP RQ), while Sr isotopic compositions were measured using TIMS (Thermo Scientific Triton Plus) at the Centre for Earth Sciences, IISc, Bengaluru. The external reproducibility for δ88Sr measurements using an 84Sr-87Sr double-spike technique [4] was better than 0.033‰ (2SD) based on repeated analyses of NIST SRM-987 Sr standard (n=6).

The δ88Sr values of the Lonar crater rocks are the first such values reported for any impact crater; the δ88Sr values range from 0.256‰ to 0.305‰ for the target basalts (average = 0.278 ± 0.04‰ (2SD), n = 6) and from 0.113‰ to 0.288‰ for the impact melt breccias. The impactites are categorized into two groups: Group 1 (n=4) with δ88Sr values overlapping those of target basalts, and Group 2 (n=5), which exhibits lower δ88Sr values relative to the target basalts. The 87Sr/86Sr ratios of the impactites (0.707519-0.708139) are more radiogenic than the target basalt average of 0.706600 and are consistent with a 3-5 wt% contribution from the underlying granitic basement of Deccan lavas to the impact melt breccias [2,3]. After correcting for the contribution of the basement, the δ88Sr values of the impactites were used to model the extent and nature of kinetic isotope fractionation, employing the standard Rayleigh fractionation model using a Monte Carlo simulation. The absence of heavier δ⁸⁸Sr values in the impact melt breccias suggests that Lonar impactites predominantly reflect origin from vapour condensates. The primary vapour originated from complete volatilization of Sr from the target and projectile, yielding a δ⁸⁸Sr similar to Lonar basalts. Group 2 impact melt breccias likely contain a component formed through nearly complete (>99%) Sr condensation within the impact vapour plume. In contrast, Group 1 impact melt breccias may have originated from the impact ejecta blanket, reflecting no evidence of significant evaporative loss.

[1] Fredriksson, K., et al. (1973), Science 180.4088.

[2] Gupta, R. D., et al. (2017), GCA, 215.

[3] Chakrabarti, R., & Basu, A.R. (2006), EPSL 247.3-4.

[4] Ganguly, S., & Chakrabarti, R. (2022), JAAS, 37(10).

How to cite: Papola, G. S. and Chakrabarti, R.: Stable Sr Variations in Impactites of Lonar Impact Crater, India: A Terrestrial Analogue for Lunar Crustal Evolution , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-630, https://doi.org/10.5194/egusphere-egu26-630, 2026.

EGU26-737 | ECS | Orals | PS1.4

 LUNAIRE - LUNAr Ionising Radiation Environment  

Bruna Lima, Tiago Neves, Luísa Arruda, Patrícia Gonçalves, António Gomes, and Marco Pinto

Characterizing the radiation environment on the lunar surface is essential for a safe human and robotic exploration. Having a negligible atmosphere, the Moon is exposed to galactic cosmic rays (GCRs), a continuous high flux of very energetic particles, and solar energetic particles (SEPs), which are accelerated in the solar corona or in coronal mass ejections. These particles can damage biological, electronic systems and other materials and thus hinder or even terminate space missions.

To aid future mission planning and habitat design, we developed a Geant4 based model, LUNAIRE, that simulates GCR and SEP propagation through the lunar surface. The model accounts for secondary particle generation on the sub-surface and derives physical quantities such as absorbed dose and Linear Energy Transfer (LET) spectrum at the surface and underground. This model was adapted from the detailed Mars Energetic Radiation Environment (dMEREM) developed by LIP (Laboratory of Instrumentation and Experimental Particle Physics) for ESA (European Space Agency), and includes location dependent surface composition, as well as user custom particle spectra as inputs.

We validated the model by comparing the LET (Linear Energy Transfer) spectrum obtained with LUNAIRE to measurements of the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) aboard the Lunar Reconnaissance Orbiter (LRO). Additionally, we compared the spectrum of secondary particles production with those of the HZETRN (High Charge and Energy Transport) code available through OLTARIS (On-Line Tool for the Assessment of Radiation in Space).

 The results allow for a reconstructed GCR spectra that matches BadhwarO'Neill (BON) Galactic Cosmic Ray Model reference curves across species. We found the LET spectrum to be in good agreement with CRaTER data for both July 2009 (solar minimum available) and July 2015 (solar maximum available). Secondary particle fluxes also match HZETRN results for neutrons and protons but are not so according for electrons and gamma particles. This was attributed to differences in the physics processes of HZETRN comparing to Geant4.

 These results show that LUNAIRE accurately characterizes the lunar radiation environment that can lead to better forecasts of, and safer missions. Ongoing work includes the evaluation against SEP events, the incorporation of complex topography geometries and validation against other mission results.

How to cite: Lima, B., Neves, T., Arruda, L., Gonçalves, P., Gomes, A., and Pinto, M.:  LUNAIRE - LUNAr Ionising Radiation Environment , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-737, https://doi.org/10.5194/egusphere-egu26-737, 2026.

EGU26-860 | ECS | Posters on site | PS1.4

Hemispheric Thermal Dichotomy in the Lunar Mantle 

Prachi Kar and Mingming Li

The Moon is thought to have solidified from a global lunar magma ocean (LMO) through fractional crystallization. Well-documented hemispheric asymmetries in topography, crustal thickness, surface abundances of radiogenic elements, and volcanic history suggest that the nearside and farside underwent distinct evolutionary pathways. These differences likely reflect variations in the deep interior, particularly in the distribution of radiogenic heat-producing elements (HPEs) capable of sustaining long-lived temperature contrasts. However, direct geophysical evidence for such a dichotomy has been limited. A recent study based on tidal response by Park et al. (2025) reveals a 2-3% difference in shear modulus between the nearside and farside mantle, implying that the nearside mantle remains ~200 K warmer today. Similarly, He et al. (2025), using Chang’e-6 farside basalt samples combined with remote-sensing-based geochemical modeling, report farside mantle temperatures at least ~100°C cooler than those of the nearside. In this study, we employ numerical modeling to investigate whether a hemispheric thermal contrast of several hundred kelvins in the lunar mantle can persist throughout lunar history and to assess how degree-1 mantle convection and HPE distributions influence the maintenance of this dichotomy. We further explore the role of dense ilmenite-bearing cumulates (IBCs), initially crystallized beneath the crust during the final stages of LMO solidification, and later overturned and settled near the core-mantle boundary due to gravitational instability, to shape the Moon’s long-term thermochemical and dynamical evolution.

How to cite: Kar, P. and Li, M.: Hemispheric Thermal Dichotomy in the Lunar Mantle, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-860, https://doi.org/10.5194/egusphere-egu26-860, 2026.

EGU26-956 | Posters on site | PS1.4

Spectral Investigation of the Mare Australe Basalts: A Fresh look at the Atypical Volcanism on the Moon 

Neha Panwar, Tvisha Kapadia, and Neeraj Srivastava

Mare Australe (47.77°S, 91.99°E) is a distinctive volcanic province (diameter ~1000km) at the eastern nearside and farside boundary of the Moon. The basalts of the region were considered a part of mare filling volcanism inside an ‘Australe Basin’ due to the circular arrangement of its 248 basaltic patches [1]. The proposed Australe Basin, however, lacks any discernible topographic signatures, a ring morphology, and a central positive Bouguer anomaly typically associated with the lunar impact basins. The results from the GRAIL mission and geological investigations revealed the presence of a ~880 km diameter impact structure in the northern part of Mare Australe, naming it the Australe North Basin (35.5°S, 96°E) [2, 3]. The Mare Australe basalts are dominantly emplaced outside this newly discovered Australe North Basin, which is perplexing. In this study, we carry out an extensive compositional investigation of the previously uncharacterized Australe region using hyperspectral data from the Moon Mineralogical Mapper (M3) onboard Chandrayaan-1. We investigate both mare and non-mare units in the region to understand their mineralogy in the given geological context. The spectral investigation reveals that despite widespread volcanism, the region lacks the presence of high-Ca pyroxene. Instead, the basalts are primarily composed of low to intermediate Ca-pyroxene in comparison to the rest of the lunar basalts, displaying their unique mineralogical signature. These findings provide new insights into the nature and origin of the atypical volcanism on the Moon in the Australe Region and highlight the distinct geological environment of Mare Australe responsible for the same. This study offers important implications for understanding lunar volcanic evolution and its relationship with impact processes.

[1] Whitford-Stark, J. L. (1979) LPSC X, 2975- 2994. [2] Neumann G. A. et al. (2015) Sci Adv. 1(9), e1500852. [3] Panwar N. and Srivastava N. (2024) Icarus, 408, 115841

How to cite: Panwar, N., Kapadia, T., and Srivastava, N.: Spectral Investigation of the Mare Australe Basalts: A Fresh look at the Atypical Volcanism on the Moon, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-956, https://doi.org/10.5194/egusphere-egu26-956, 2026.

EGU26-2285 | ECS | Orals | PS1.4

Magmatic origin of the Dewar magnetic anomaly: Implications for an early lunar dynamo 

Xi Yang, Anna Mittelholz, Adrien Broquet, and Max Moorkamp

The Moon’s ancient magnetic field provides critical insights into its thermal and magnetic evolution, yet the lifetime of its dynamo remains debated. Returned samples yield complex and contradictory paleomagnetic records, while orbital data reveal crustal magnetic anomalies of uncertain origin from either a core dynamo or transient impact-generated fields. Here we jointly invert gravity and magnetic observations in the region around the Dewar swirl, a high-albedo feature associated with the Dewar magnetic anomaly. We identify a shallow, magnetized, high-density body consistent with buried mare basalt. Its formation requires paleointensity exceeding 11 μT, suggesting a lunar dynamo was active at about 4.2 Ga, as constrained by the superposed basin ejecta. Results also show that swirl formation requires horizontal magnetization and iron oxide enrichment. These findings link a magnetic anomaly to its geologic source and the state of the lunar dynamo, providing new constraints on the lunar magnetic and volcanic history.

How to cite: Yang, X., Mittelholz, A., Broquet, A., and Moorkamp, M.: Magmatic origin of the Dewar magnetic anomaly: Implications for an early lunar dynamo, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2285, https://doi.org/10.5194/egusphere-egu26-2285, 2026.

Reliable assessment of lunar surface engineering behavior requires regolith simulants that realistically capture both the mechanical response and impact-derived characteristics of natural lunar regolith. Although numerous lunar regolith simulants have been developed for geotechnical testing, most remain insufficient in reproducing the structure and mechanical role of impact products such as agglutinates and impact breccias, which dominate the load-bearing framework of lunar regolith. In this study, we establish a fabrication route for lunar regolith simulants that combines thermal processing of basalt-derived materials with glass-phase incorporation and subsequent mechanical crushing. Using this method, two simulant series, THIP-5 and THIP-6, are designed to represent regolith conditions at the Chang’e-5 nearside and Chang’e-6 farside landing regions, respectively. Systematic laboratory characterization demonstrates that the impact product simulant generated with 25 wt.% hollow glass beads reproduce key morphological and micromechanical features of natural lunar impact products. Comparisons of bulk scale properties further reveal that the synthesized simulants closely match their corresponding target soils across multiple physical and compositional metrics, including mineralogy, chemistry, grain-size characteristics, and density-related parameters. Furthermore, static angle of repose tests show that THIP-5 exhibits behavior comparable to established Chang’e-5 simulants, while experimental results from THIP-6 enable an estimation of the static angle of repose of the Chang’e-6 regolith at approximately 52.8°. The THIP simulant framework provides a physically grounded experimental basis for investigating lunar regolith mechanics, supporting the design of surface infrastructure, mobility systems, and future astronaut operations on the Moon.

How to cite: Luo, A., Cui, Y., and Nie, J.: Lunar regolith simulants incorporating impact product simulants for surface engineering and exploration applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2442, https://doi.org/10.5194/egusphere-egu26-2442, 2026.

EGU26-3498 | ECS | Posters on site | PS1.4

Mineralogical Diversity and Crustal Composition of Selected Lunar Regions Based on M³ Hyperspectral Analysis: Implications for ISRU and Future Exploration 

Clara Guth, Francesca Mancini, Pascal Allemand, Francesco Salese, and Gian Gabriele Ori

Characterizing lunar surface mineralogy is essential for understanding crustal evolution, magma ocean differentiation, impact excavation processes, and identifying In-Situ Resource Utilization (ISRU) targets for future exploration. This study determines the mineralogical composition and crustal stratigraphy across four geologically distinct lunar terrains using Moon Mineralogy Mapper (M³) hyperspectral data: the Aristarchus plateau (volcanically complex), Dionysius crater (a pristine impact structure), the Malapert region (ancient highlands of the South Pole), and Leibnitz R (primordial anorthositic crust).

Level-2 M³ hyperspectral cubes (430-3000 nm, 140 m/pixel) [1] were processed through systematic workflows: destriping, photometric normalization, Minimum Noise Fraction (MNF) transform, Pixel Purity Index (PPI) endmember extraction, continuum removal, and Spectral Angle Mapper (SAM) classification. Spectral signatures were validated against RELAB laboratory spectra resampled to M³ resolution. Key mineral phases identified include anorthite, low-calcium pyroxene (LCP), high-calcium pyroxene (HCP), olivine, spinel-bearing assemblages, and ilmenite.

Aristarchus exhibits the highest mineralogical diversity [2], with anorthositic highland material, HCP- and LCP-bearing mafic units, and localized olivine signatures. Anorthosite absorption features (1.25 µm band depth) dominate the crater floor, pyroxene signatures characterize the ejecta blanket, and olivine (1 µm band depth) appears along crater rims. This heterogeneity reflects volcanic emplacement and deep impact excavation, offering diverse oxygen-rich and iron-bearing ISRU targets.

Dionysius (Mare Tranquillitatis) reveals systematic radial mineralogical zonation from HCP-dominated rim materials to LCP-enriched central exposures, indicating excavation through compositionally stratified crust. This vertical gradient constrains upper crustal HCP overlying lower crustal LCP layers [3,4], consistent with magma ocean crystallization models. Olivine and ilmenite detections suggest penetration to mafic lithologies, constraining crust-mantle differentiation.

Malapert (South Pole) is predominantly anorthositic, with isolated spinel-bearing outcrops (5% band depth at 2 µm) associated with uplifted crustal blocks. These exposures constrain deep crustal composition and early magma ocean differentiation. The area's abundant anorthosite and its location near permanently shadowed regions make it key site for oxygen extraction and the establishment of polar exploration facilities.

Leibnitz R (far side) displays spectrally pure anorthositic composition, representing primordial crust formed during lunar magma ocean plagioclase flotation. Its compositional homogeneity provides a reference for early lunar differentiation and high-purity feedstock for ISRU oxygen production.

This study integrates hyperspectral mineralogy with surface morphology to constrain crustal architecture and geological evolution across diverse lunar environments. The methodology establishes a replicable framework for hyperspectral analysis applicable to future mission planning, linking fundamental crustal processes to ISRU resource assessment and advancing sustainable lunar exploration strategies.

References: [1] Green et al. (2011) JGR: Planets, 10.1029/2011JE003797; [2] Chevrel et al. (2009) Icarus, 10.1016/j.icarus.2008.08.005; [3] Moriarty & Pieters (2018) JGR, 10.1002/2017JE005364; [4] Wieczorek et al. (2013) Science, 10.1126/science.1231530

Acknowledgement: EU HORIZON-MSCA-2023-SE-01, Grant 101183089

How to cite: Guth, C., Mancini, F., Allemand, P., Salese, F., and Ori, G. G.: Mineralogical Diversity and Crustal Composition of Selected Lunar Regions Based on M³ Hyperspectral Analysis: Implications for ISRU and Future Exploration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3498, https://doi.org/10.5194/egusphere-egu26-3498, 2026.

With the advancement of deep space exploration, conducting electromagnetic (EM) sounding on the Moon is of great significance for investigating the lunar internal structure and the surface EM environment. Since the Moon lacks a global dipole magnetic field and is directly exposed to complex solar wind and Earth's magnetotail environments, clarifying its time-domain response mechanisms to external magnetic perturbations is a prerequisite for lunar surface EM exploration.

This study establishes a homogeneous spherical model to simulate the lunar electromagnetic response to disturbances in the interplanetary magnetic field. By deriving analytical solutions for electromagnetic fields under step excitation (simulating a 10 nT abrupt change in the solar wind), the transient response characteristics for lunar internal electrical conductivities in the range of 10-5 ~10-7S/m are quantitatively analyzed.

The simulation results reveal distinct induction mechanisms:(1) The penetration of the magnetic field is governed by the skin effect. Higher conductivity leads to a stronger shielding effect and a longer rise time to reach the steady state, whereas lower conductivity allows for faster magnetic propagation. (2) The induced electric field exhibits a transient response, with its magnitude inversely proportional to conductivity. Lower conductivity results in a higher instantaneous peak electric field but a faster decay, while higher conductivity suppresses the peak amplitude but extends the signal duration. (3) The induced electric field displays a toroidal symmetry along the latitudes, reaching its maximum at the lunar equator and zero at the poles, with no vertical component.

These findings indicate that electric field detection is particularly suitable for capturing high-frequency transient variations. The derived relationships between signal bandwidth, field intensity, and conductivity provide a theoretical reference for future lunar electromagnetic exploration.

How to cite: Zhang, W., Wang, Z., and Liu, Z.: Time-Domain Simulation and Transient Characteristics of Induced Electromagnetic Fields for Lunar Deep Interior Sounding, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3527, https://doi.org/10.5194/egusphere-egu26-3527, 2026.

EGU26-3637 | Orals | PS1.4

L-MAG: A Temperature-Stabilized Fluxgate Magnetometer System for Long-Term Lunar Surface Observatories 

Hao Cao, Robert Strangeway, Krishan Khurana, Ryan Caron, Emil McDowell, David Pierce, David Hinkley, and Natalie Walsh

Lunar magnetic field investigation connects the interior, the surface, and the space environment of the Moon. Measuring and understanding the lunar magnetic field at different length-scales and time-scales is of critical importance to understand the bulk water content and temperature profile in the lunar mantle, the existence and properties of a partial melt layer above the lunar core, the size of the lunar core, the origin of volatiles on the lunar surface, and the origin and properties of the past lunar dynamo, all of which are intimately connected to the origin of the Earth-Moon system and the subsequent thermal-chemical-environmental evolution of the Moon. The surface of the Moon, however, is a challenging environment, including contrasting temperatures between lunar day and lunar night, dust, and surface charging.

 

Here we report our progress in the designing, building, and testing of a temperature-stabilized fluxgate magnetometer (FGM) system for long-term operations on the surface of the Moon. We refer to this FGM system configuration as L-MAG. The sensor design draws heritage from those onboard the NASA Magnetospheric Multiscale (MMS) mission, InSight Mars Lander, the Europa Clipper mission, and most recently the TRACERS mission. One of the key improvements is a magnetically clean AC heater that directly surrounds the FGM sensor, improving power efficiency and responsiveness compared to Europa Clipper Magnetometer’s distant heater pod. Thermal losses are reduced with a low-emissivity enclosure and lightweight Kapton flex harness. The heater system is designed to yield a temperature stability of ± 0.1 degrees °C around two set-point temperatures (day and night) to further reduce long-term drift, allowing the inference of lunar induction responses at periods of  105 seconds and longer, necessary to probe the lower lunar mantle and core. This power efficient FGM design will be compatible with installation onto a lunar lander or placed on the surface of the moon by an astronaut. Our L-MAG system will significantly improve measurement capabilities for upcoming lunar science missions including those via the Commercial Lunar Payload Services (CLPS) and via Artemis astronaut deployments.

How to cite: Cao, H., Strangeway, R., Khurana, K., Caron, R., McDowell, E., Pierce, D., Hinkley, D., and Walsh, N.: L-MAG: A Temperature-Stabilized Fluxgate Magnetometer System for Long-Term Lunar Surface Observatories, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3637, https://doi.org/10.5194/egusphere-egu26-3637, 2026.

EGU26-5115 | Posters on site | PS1.4

LUNINA: In‑situ Navigation and Communication Infrastructure for Lunar Science 

Harri Haukka, Antti Kestilä, Ari-Matti Harri, Maria Genzer, Leo Nyman, Petri Koskimaa, and Jarmo Kivekäs

Introduction and heritage

LUNINA is a compact, durable, and location‑independent node that provides accurate navigation and communication services on the Moon. Based on the FMI led ESA’s MiniPINS/LINS project heritage, each LUNINA unit operates autonomously nominally with RHU‑assisted thermal control, solar power, and batteries. RTG-unit option is also available. Deployed individually or as a network, LUNINA nodes enables precise positioning, robust data relay, and continuous operations, enabling and supporting the scientific missions on Moon surface and orbital missions. 

Future Lunar science and missions requires dependable surface infrastructure for positioning and communication (data etc.). While future Lunar constellations will provide space segment navigation, surface users will face line‑of‑sight constraints, topographic shadowing etc. obstacles, and Lunar thermal extremes. LUNINA addresses these challenges with a drop‑and‑forget node that include navigation aid option and provides local data relay for science operations.

Figure: LUNINA nodes on the Lunar surface. Network of LUNINA's form an Earth-like mobile communication grid that supports both human and robotic Lunar exploration.

Surface operations that support the Lunar science

Accurate positioning supports the scientific operations, and it is required to achieve requirements posed by each Lunar mission goals. Nodes establish a resilient, low‑latency link between e.g. sensors/instruments, rovers, habitats, and orbiters. This LUNINA link capability and feature supports high efficiency measurements (e.g. done by multiple individual dust/plasma, thermal, environmental monitoring stations) and provides a 24/7 operating safety and communication channel for EVA operations as well. RHU‑assisted LUNINA thermal control maintains electronics safe through the Lunar night, reducing data loss and enabling long time‑series measurements and observations essential for understanding e.g. Lunar regolith thermophysics, exosphere variability, and electrostatic dust rising practically in all possible locations on Moon where at least some Sun light is present for solar panels. If node is equiped with optional RTG-unit providing the required power, then node is location-independent. In addition to this, strategic placement on hills or crater rims extends line‑of‑sight coverage into otherwise inaccessible terrain, complementing the Lunar Communications and Navigation Services (LCNS) space segment when available. We have identified following main science use cases for LUNINA:

  • Geophysics: seismic science instrumentation as a piggy-back of LUNINA node. Delivery of the observation telemetry for crustal structure science and impact monitoring.
  • Regolith and environment: LUNINA node assisting the thermal probes and permittivity sensors with nighttime power/thermal survivability in heat flow and volatile behaviour research.
  • Dust–plasma interactions: electric field, plasma, and dust sensors included as a piggy-back at multiple LUNINA nodes to resolve charging and dust rising dynamics.
  • Resources search and identification: navigation and data relay assist for mapping of the terrain that are in shadowed regions from Moon base and/or main lander.

Conclusions

LUNINA provides practically the nonstop navigation and communications base infrastructure that Lunar science needs and it is easy to scale with additional nodes. By enabling precise positioning, robust data relay, and night‑survivable operations, LUNINA contributes to the achieving of Lunar scientific benefits and results and supports both robotic and human Lunar exploration.

How to cite: Haukka, H., Kestilä, A., Harri, A.-M., Genzer, M., Nyman, L., Koskimaa, P., and Kivekäs, J.: LUNINA: In‑situ Navigation and Communication Infrastructure for Lunar Science, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5115, https://doi.org/10.5194/egusphere-egu26-5115, 2026.

EGU26-5708 | Posters on site | PS1.4

Mineralogical, Geochemical and Chronological Study of the lunar fragmental breccia Pakepake_005 

Cheng Yue, Xiaochao Che, Tao Long, Ziyao Wang, Ming Jin, Xiaozhong Ding, Qian Ma, and Dunyi Liu

Pakepake_005 is a lunar fragmental breccia recovered from the Taklamakan Desert, Xinjiang, China. It exhibits a clastic breccia texture, in which mineral fragments and subordinate lithic clasts are cemented by matrix and impact glass. The dominant phases are plagioclase and pyroxene, whereas olivine is less abundant but widely distributed. Minor to accessory phases include ilmenite, chromite, troilite, phosphates, silica, baddeleyite, armalcolite, and Fe–Ni metal. Lithic clasts comprise impact-melt, plutonic, and basaltic components, as well as symplectites produced by breakdown of pyroxene.

Pyroxene clasts are predominantly subhedral to anhedral and range from ~0.1 to 1 mm in size. A subset exhibits fine clinopyroxene–orthopyroxene exsolution lamellae, with Mg# spanning 15.3–71.4 and locally well-developed Fe–Mg zoning. In contrast, some Fe-rich pyroxenes lack exsolution, are compositionally homogeneous, commonly fractured, and have Mg# values of 6.6–45.2. Some Fe-rich pyroxenes underwent breakdown reactions to form symplectites consisting of augite (Mg# = 30.7–35.5), fayalitic olivine, and quartz, accompanied by minor ilmenite and phosphate minerals. Mg-rich pyroxenes also lack exsolution, are comparatively homogeneous, and have Mg# values of 50.7–74.8.

Pyroxene compositions define two distinct populations on the Fe/(Fe+Mg)–Ti/(Ti+Cr) diagram, indicating multiple sources. The first group shows a positive correlation between Fe/(Fe+Mg) and Ti/(Ti+Cr), consistent with pyroxenes from very low-Ti (VLT) lunar basalts [1]. The second group is characterized by higher Mg# together with relatively elevated Ti/(Ti+Cr), consistent with magnesian pyroxenes crystallized from a more primitive melt. CI-chondrite-normalized REE patterns [2] further indicate that those pyroxenes record at least two sources.

In situ SHRIMP U–Pb geochronology of phosphates and baddeleyite from different components constrains two major events recorded by Pakepake_005. Phosphates hosted in the matrix and impact-derived lithic clasts yield an impact age of 3923 Ma, consistent with the Imbrium basin forming event around ~3.9 Ga[3]. In contrast, phosphates in symplectites and baddeleyite from a VLT clast yield an age of 3486 Ma, documenting a VLT magmatic episode. Taken together, these petrographic, mineral-chemical, and chronological constraints suggest that Pakepake_005 was sourced from an Imbrium-ejecta–related VLT basaltic unit, broadly analogous to basaltic materials exposed in the northern Mare Imbrium region (e.g., east of the Chang’e-3 landing site), where remote-sensing data indicate VLT compositions and yield model eruption ages of ~3.5 Ga for the associated basaltic unit [4].

Acknowledgments: This study was financially supported by National Key R&D Program of China from Ministry of Science and Technology of the People’s Republic of China grant no. 2022YFF0704905, the National Natural Science Foundation of China (NSFC) grant no. 42241107 and the Open Project for Innovative Platform of Meteoritical Research, Shanghai Science and Technology Museum.

[1] Robinson K. L. et al. (2012). Meteoritics & Planetary Science 47: 387–399.[2] Anders E. and Grevesse N. (1989). Geochimica et Cosmochimica Acta 53: 197–214.[3] Nemchin A. A. et al. (2021). Geochemistry 81: 125683.[4] Ji J. et al. (2022). Science Bulletin 67: 1544–1548.

How to cite: Yue, C., Che, X., Long, T., Wang, Z., Jin, M., Ding, X., Ma, Q., and Liu, D.: Mineralogical, Geochemical and Chronological Study of the lunar fragmental breccia Pakepake_005, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5708, https://doi.org/10.5194/egusphere-egu26-5708, 2026.

EGU26-6066 | Orals | PS1.4 | Highlight

First robotic attempt to measure heat flow of the Moon: Deployment of LISTER on Blue Ghost Mission One to Mare Crisium 

Seiichi Nagihara, Kris Zacny, Peter Ngo, Luke Sanasarian, Roshan Misra, Matthias Grott, Joerg Knollenberg, Suzanne Smrekar, Matthew Siegler, and Clive Neal

On March 2, 2025, Firefly Aerospace became the first United States-based company to successfully soft-land a robotic spacecraft on the Moon. The Blue Ghost lander deployed all 10 NASA-supported payloads under the Commercial Lunar Payload Services. The Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity (LISTER) was one of them. LISTER measured temperature and thermal conductivity of the lunar regolith of the landing site at 8 depths down to 1 m for the purpose of quantifying the endogenic heat flow of the Moon. To penetrate to the subsurface, LISTER used the pneumatic excavation technique in which the deployment mechanism spooled out a 6.4-mm diameter stainless steel tube and blew pressurized nitrogen gas through a nozzle attached to the leading end of the tube.  The gas jet, rapidly expanding in the lunar vacuum, removed the regolith ahead of the nozzle, while the spooling motor applied weight to advance deeper into the subsurface. The thermal sensors were encased in a stainless-steel needle, 28-mm long and 2.8-mm diameter, attached to the gas nozzle. When the needle sensor reached a depth targeted for thermal measurements, LISTER stopped the gas jet and inserted the needle into the bottom-hole regolith. Each thermal measurement sequence took 2 hours. During the first hour, the needle thermally equilibrated with the regolith. Then, the needle was electrically heated with a constant power of 50 mW for 30 minutes, followed by a 30-minute cool-off period. Thermal conductivity of the regolith was determined by modeling the rise and fall of the needle temperature during the 2nd hour using a finite-element heat transfer model.

Prior to the mission, it was hoped that LISTER would reach greater than 1-m depth into the subsurface, where temperature of the regolith is not significantly affected by the insolation cycles.  Then, the endogenic heat flow would have been obtained simply as the product of the thermal gradient and the thermal conductivity of the regolith depth interval penetrated. Because LISTER did not reach that depth, the heat flow is being determined as the lower boundary condition for a one-dimensional (vertical) finite-element heat transport model that simulates the interaction between the upward flow of the endogenic heat and the downward propagation of the insolation-induced thermal waves. The history of the insolation-induced surface temperature swings at the landing site, which is the surface boundary condition for the heat transport model, has been reconstructed from the ephemeris of the landing site and surface temperatures determined from flyovers by the Diviner radiometer onboard the Lunar Reconnaissance Orbiter. The equilibrium temperature and thermal conductivity of the regolith determined at 8 depths by LISTER provide key constraints to the model. Our early results suggest endogenic heat flow values of 13 to 14 mW/m2, comparable to what was observed at the Apollo 17 site (16 mW/m2). A more thorough inversion is now being carried out to optimize the heat flow determination and estimate its uncertainty.

How to cite: Nagihara, S., Zacny, K., Ngo, P., Sanasarian, L., Misra, R., Grott, M., Knollenberg, J., Smrekar, S., Siegler, M., and Neal, C.: First robotic attempt to measure heat flow of the Moon: Deployment of LISTER on Blue Ghost Mission One to Mare Crisium, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6066, https://doi.org/10.5194/egusphere-egu26-6066, 2026.

Accurate knowledge of the lunar gravitational field is essential for lunar exploration, for instance, for gravity predictions at prospective landing sites, for inertial navigation or to establish a physically meaningful height system. This contribution presents a new suite of Lunar Gravitational Maps 2026 (LGM2026). LGM2026 is sampled at the resolution of 128 pixels per degree (~250 m at the equator) and surpasses LGM2011, the most detailed lunar surface gravitational model to date, by a factor of ~6. The 250-m resolution was reached by combining long-wavelength gravity observed by the GRAIL satellites (scales up to 11 km at the equator) with short-scale gravity inferred from LRO and Kaguya topography (scales from 11 km to 250 m). To make the modelling of short-scale signals realistic, LGM2026 relies on a 3D crustal density model as opposed to the constant-density assumption of LGM2011. LGM2026 depicts (i) the gravitational potential (useful for studying gravity-driven mass movements or flow direction of fluids), (ii) the full gravitational vector (gravity predictions at landing sites, inertial navigation, verification of accelerometer readings) and (iii) the full gravitational tensor (upward/downward continuation of the potential and vector data, spacecraft navigation). The maps shows the gravitational field at the lunar surface and on a sphere of the radius 1749 km passing outside of all masses. As a by-product, LGM2026 was converted into a series of external spherical harmonics up to degree 11,519. The purpose of LGM2026 is to provide a high-resolution gravitational model for applications that are sensitive to the variations of the lunar gravitational field such as gravity predictions at landing sites or inertial navigation. Given that the short-scale signals are derived from the topography instead of gravity observations, LGM2026 must not be geophysically or geologically interpreted at scales smaller than 11 km. The accuracy of LGM2026 is estimated to 2 mGal in terms of the gravitational vector. All LGM2026 maps use the principal axes coordinate system. The release of LGM2026 is scheduled to mid-2026. This work was funded by the EU NextGenerationEU through the Recovery and Resilience Plan for Slovakia under the project No. 09I03-03-V04-00273.

How to cite: Bucha, B.: 250-m resolution lunar gravitational maps from gravity observed by satellites and gravity modelled from topography and 3D crustal density, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6331, https://doi.org/10.5194/egusphere-egu26-6331, 2026.

EGU26-6654 | ECS | Orals | PS1.4

In situ Rb–Sr geochronology and geochemistry to constrain lunar volcanism 

Rico Fausch, F. Scott Anderson, Audrey E. Aebi, Amanda M. Alexander, Edward B. Bierhaus, Sarah E. Braden, Amy L. Fagan, Sierra N. Ferguson, James W. Head III, Alex M. Iseli, Katherine H. Joy, Julie M. Korsmeyer, Jonathan Levine, Steven Osterman, John F. Pernet-Fisher, Vishaal Singh, Romain Tartèse, Tina L. Teichmann, Peter Wurz, and Marcella A. Yant

The Chemistry, Organics and Dating Experiment (CODEX) is a compact, dual-mode laser-ablation time-of-flight mass spectrometer developed for the DIMPLE payload (CLPS CP-32) to provide co-registered geochemical context and in situ Rb–Sr chronometry on the lunar surface. DIMPLE targets Ina, among the largest irregular mare patches (IMPs), to test whether IMPs record geologically recent volcanism or instead reflect ancient, highly vesicular basaltic deposits with poor small-crater preservation. Absolute ages tied to measured composition are required because morphology and crater statistics alone are ambiguous for these terrains. The CODEX architecture couples 266 nm UV laser-ablation mass spectrometry (LAMS) for major and trace-element mapping (m/z 1–250) with laser-ablation resonance-ionization mass spectrometry (LARIMS) for selective, interference-free Rb and Sr isotope measurements that mitigate the 87Rb/87Sr isobar without relying on extreme mass resolving power. We are currently commissioning the CODEX Engineering Development Unit (EDU). First LAMS measurements on calibration samples show m/Δm ≈ 300–400 (FWHM) across the targeted range and clear isotopic structure (e.g., resolved Fe and Pb isotopes), indicating robust transmission and margin for compositional mapping. Ongoing work is extending these EDU results toward resonance-ionization operation to validate the end-to-end Rb–Sr measurement chain and quantify isotope performance under representative conditions.

How to cite: Fausch, R., Anderson, F. S., Aebi, A. E., Alexander, A. M., Bierhaus, E. B., Braden, S. E., Fagan, A. L., Ferguson, S. N., Head III, J. W., Iseli, A. M., Joy, K. H., Korsmeyer, J. M., Levine, J., Osterman, S., Pernet-Fisher, J. F., Singh, V., Tartèse, R., Teichmann, T. L., Wurz, P., and Yant, M. A.: In situ Rb–Sr geochronology and geochemistry to constrain lunar volcanism, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6654, https://doi.org/10.5194/egusphere-egu26-6654, 2026.

EGU26-7444 | Posters on site | PS1.4

The Twin Impact Lunar Telescope network 

Marco Delbo, Philippe Lognonne, Paul Girard, Nicolas Mauclert, Daniel Sheward, Chrysa Avdellidou, Laurent Herrier, Thierry Parra, Jean-Pierre Rivet, Bruno Mongellaz, Nicolas Anfosso, Enguerrand Maeght, Didier Grimaldi, Pierre-Yves Froissart, Christelle Saliby, Andrea Ferrero, and Marco Angelini
Lunar impact flashes (LIFs) provide direct constraints on the flux and physical properties of meteoroids impacting the Earth–Moon system. Conventional LIF monitoring, performed mainly in the visible wavelength range, is strongly limited by lunar phase, sky brightness, and observing geometry, resulting in sparse temporal coverage and a low probability of detecting rare, high-energy events.
 
The Twin Impact Lunar Telescope (TILT) has been developed to overcome these limitations through a dedicated instrumental concept combined with a global observing strategy. Three telescopes will be deployed worldwide in the frame of the LISTEN FLASH ERC project. Each TILT node consists of two co-aligned telescopes optimized for high-cadence lunar observations in the near-infrared (NIR), where typical LIF thermal emission (∼2500–3000 K) peaks. Observations in the J band (~1.2 μm) benefit from increased photon flux and reduced atmospheric scattering compared to visible bands, enabling effective monitoring under bright sky conditions, including twilight and daytime. Simultaneous observations with twin telescopes allow robust discrimination between real lunar impact flashes and false positives, while a geographically distributed network of TILT stations provides near-continuous lunar coverage and redundancy against local observing constraints.
 
We present the TILT system design, observational strategy, and expected performance in terms of detection rates and impact energy thresholds. We also highlight the synergy of the TILT network with the lunar seismic experiments scheduled between 2026 and 2030. The TILT well-timed and located impacts will indeed provide known sources, enabling a direct computation of the seismic travel times for each pair of TILT LIF records and seismic records. This data set will  constraints on the thickness of the lunar crust and its early evolution.

 

The TILT-1, installed at the Observatory of Calern (Observatoire de la Côte d'Azur) was sucesfully tested during the Geminids meteor shower in December 2025. Recording of some tens of potential LIF, several of which being confrimed, was achieved. 

How to cite: Delbo, M., Lognonne, P., Girard, P., Mauclert, N., Sheward, D., Avdellidou, C., Herrier, L., Parra, T., Rivet, J.-P., Mongellaz, B., Anfosso, N., Maeght, E., Grimaldi, D., Froissart, P.-Y., Saliby, C., Ferrero, A., and Angelini, M.: The Twin Impact Lunar Telescope network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7444, https://doi.org/10.5194/egusphere-egu26-7444, 2026.

EGU26-8051 | ECS | Orals | PS1.4

Electrostatic-driven method for lunar regolith sampling 

Serena R. M. Pirrone, Trunal Patil, Jarrett Dillenburger, Abhimanyu Shanbhag, and Kathryn Hadler

In Situ Resource Utilization (ISRU) is being proposed as the strategy to establish long-term presence on the Moon and to facilitate future crewed missions farther, e.g., Mars, thanks to the creation of products by using local resources [1]. Due to its composition and physical characteristics, lunar regolith represents a key resource for human life support, propellant production, and the construction of infrastructures [2-4]. The development of efficient regolith sampling technologies hence represents a crucial first step to increase our understanding of lunar resources. Within the previous exploration missions on the Moon and recent technology developments, several approached have been proposed for the collection of regolith [5]. There has been great attention in optimizing technology performance, however developing systems capable of acquiring regolith samples that are representative of the sampled region is still a necessity [5].

The present work proposes the design, development and testing of a system employing electrostatic and vibration forces to execute a precise and representative sampling of surface lunar regolith. The sampling system was tested at controlled relative humidity conditions at the European Space Resources Innovation Centre (ESRIC) in Luxembourg. Samples of LHS-1 lunar regolith simulant with changing compaction levels were created using air pluviation technique as previously done in [6]. Our findings showed greater regolith collection for LHS-1 samples with lower initial porosity. Sampling performance was also evaluated with changing environment relative humidity (RH) conditions showing greater regolith collection with decreasing RH for values below 18 %, after which it was constant. In addition, how sampling performance is affected by the process duration was investigated resulting in greater mass collected during longer operations for processes up to 360 s, after which saturation was observed. Finally, for the first time, the Particle Size Distributions of collected and original regolith samples were measured and the mean values of particle size diameters did not show important relative differences, demonstrating the representativity of the proposed sampling system.

 

 [1] G. B. Sanders, “Advancing In Situ Resource Utilization Capabilities To Achieve a New Paradigm in Space Exploration,” in 2018 AIAA SPACE and Astronautics Forum and Exposition, Orlando, FL: American Institute of Aeronautics and Astronautics, Sep. 2018. doi: 10.2514/6.2018-5124.

[2] I. A. Crawford, “Lunar resources: A review,” Prog. Phys. Geogr. Earth Environ., vol. 39, no. 2, pp. 137–167, Apr. 2015, doi: 10.1177/0309133314567585.

[3] M. B. Duke, “Development of the Moon,” Rev. Mineral. Geochem., vol. 60, no. 1, pp. 597–655, Jan. 2006, doi: 10.2138/rmg.2006.60.6.

[4] M. Anand et al., “A brief review of chemical and mineralogical resources on the Moon and likely initial in situ resource utilization (ISRU) applications,” Planet. Space Sci., vol. 74, no. 1, pp. 42–48, Dec. 2012, doi: 10.1016/j.pss.2012.08.012.

[5] S.R.M. Pirrone et al., “Lunar Regolith Sampling Technologies: A Critical Review“, Space Sci Rev 221, 111, Nov. 2025, doi: 10.1007/s11214-025-01239-6.

[6] S.R.M. Pirrone et al., “The Effect of Tip Design on Technological Performance During the Exploration of Earth, Lunar, and Martian Soil Environments,” J. Field Robot., p. rob.70043, Aug. 2025, doi: 10.1002/rob.70043.

How to cite: Pirrone, S. R. M., Patil, T., Dillenburger, J., Shanbhag, A., and Hadler, K.: Electrostatic-driven method for lunar regolith sampling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8051, https://doi.org/10.5194/egusphere-egu26-8051, 2026.

EGU26-8506 | ECS | Orals | PS1.4

Statistical Study of Moon-originating Ions in the Solar Wind 

Jaehee Lee, Khan-Hyuk Kim, Yewon Hong, Seul-Min Baek, Ho Jin, and Junhyun Lee

When the Moon was in the solar wind, Kaguya frequently observed ions originating from the Moon. To examine their statistical properties, we analyzed Kaguya low-energy particle data obtained from January 2008 to June 2009. These Moon-originating ions were mainly detected on the lunar far side, with energies ranging from 20 to 300 eV. At the time of their creation at or near the lunar surface, the ions are expected to have energies of only a few eV or less. Consequently, the ions observed by Kaguya are energized by a factor of 10 to 100. Time-of-flight (TOF) analyses indicate that these ions consist of C+, O+, Na+, Al+, K+, and Ar+. We found a pronounced asymmetry between the Northern and Southern Hemispheres in the detection rate of Moon-originating ions. These ions are concentrated mainly at high northern latitudes. To investigate the energization and asymmetric spatial distribution of Moon-originating ions, we perform test-particle simulations and discuss where and how the ions are energized and what produces the asymmetry.

How to cite: Lee, J., Kim, K.-H., Hong, Y., Baek, S.-M., Jin, H., and Lee, J.: Statistical Study of Moon-originating Ions in the Solar Wind, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8506, https://doi.org/10.5194/egusphere-egu26-8506, 2026.

EGU26-8526 | Orals | PS1.4

Results from the Lunar Magnetotelluric Sounder on Blue Ghost Mission 1 

Catherine L. Johnson, Robert E. Grimm, Jared Espley, Ian Garrick-Bethel, Stephanie K. Howard, Rachel E. Maxwell, Clive R. Neal, and David E. Stillman

Blue Ghost Mission 1 (BGM1) landed on the Moon in Mare Crisium (18.562 °N, 61.810 °E) on March 3, 2025.  It deployed the lunar magnetotelluric sounder (LMS), the first extraterrestrial MT experiment, designed to investigate upper mantle electrical conductivity and temperature, outside the Moon’s Procellarum KREEP Terrane (PKT).  The PKT exhibits extensive mare volcanism and surficial heat-producing elements (HPE), but their causal relationship remains unclear.  Specificially, the amount and depth distribution of HPE elements beneath the PKT is unknown and various models have different implications for mantle temperature.  Mantle electrical conductivity has previously been investigated at the Apollo 12 (A12) site, and new data acquired from BGM1 provide the opportunity to compare electrical conductivity profiles and inferred mantle temperatures beneath sites inside (A12) and outside (BGM1) the PKT.

LMS operated until March 12, 2025. Comparison of vector magnetic field data from LMS and the ARTEMIS THEMIS-B orbiting spacecraft show the transit through the solar wind, the magnetosheath and the magnetotail, with bow shock crossings and the magnetotail current sheet crossing clearly observed in LMS data.

A landing site with small crustal fields was desirable for the electrical conductivity experiment to minimize plasma interactions.  Satellite-based models predict surface fields of less than 10 nT at BGM1.  Although measurement of crustal fields was not a science requirement or objective, determination of the static field has been possible and it can be demonstrated to be of primarily crustal (not spacecraft) origin.  The resulting surface field of ~65 nT reflects only modest additional contributions from magnetizations not observable from orbit.

The magnetotelluric (MT) method uses orthogonal horizontal components of local time-varying electric and magnetic fields to determine subsurface electrical conductivity. However, a combination of plasma conductivity 10x higher than expected and magnetometer placement relatively far from the surface resulted in a frequency-dependent attenuation of the induction signal. Although MT produces plausible results, we focus on electrical conductivity results obtained using the magnetic Transfer Function (TF) approach, that compares fields measured at the surface to those measured at distance from the Moon.  We compare LMS measurements at BGM1 with reference magnetic fields measured by THEMIS-B to obtain TF at BGM1, and invert these for electrical conductivity.  We also reinvert TFs computed using A12 surface fields and those measured simultaneously by the distant Explorer 35 orbiter. We find that the temperature difference between A12 and BGM1 derived from electrical conductivity is <100 K (+1-sigma level) at 200-km depth. This is incompatible with excess HPE abundances required for PKT-centric partial melting throughout lunar history. We suggest that the thin crust at PKT led to preferential eruption of mare basalts, and preferential excavation of globally distributed urKREEP. We conclude that regional volcanism and surficial incompatible elements in PKT are not genetically related.

LMS Team: R. Grimm (PI), G. Delory, J. Espley, I. Garrick-Bethel, J. Gruesbeck, S. Howard, C. Johnson, R. Maxwell, C. Neal, T. Nguyen, R. Nolan, M. Phillips, M. Purucker, D. Sheppard, F. Simpson, C. Smith, T. Smith, D. Stillman, T. Taylor, P. Turin.

How to cite: Johnson, C. L., Grimm, R. E., Espley, J., Garrick-Bethel, I., Howard, S. K., Maxwell, R. E., Neal, C. R., and Stillman, D. E.: Results from the Lunar Magnetotelluric Sounder on Blue Ghost Mission 1, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8526, https://doi.org/10.5194/egusphere-egu26-8526, 2026.

EGU26-8775 | ECS | Posters on site | PS1.4

Interaction Between Solar Wind Particles and the Reiner Gamma Magnetic Anomaly: Observations and Test-Particle Simulations 

Yewon Hong, Khan-Hyuk Kim, Jaehee Lee, Ho Jin, and Seul-Min Baek

Some lunar crustal magnetic anomalies are associated with albedo markings known as swirls; however, the processes governing their formation remain unclear. In this study, we focus on Reiner Gamma, a well-studied lunar anomaly and a key site for investigating the relationship between albedo patterns and magnetic anomalies. We perform test-particle simulations to examine how the Reiner Gamma swirl interacts with the local magnetic field, employing incident solar wind particles with energies of 0.5–1.0 keV and both line and disk magnetization models. The simulated magnetic fields are comparable to observations from previous lunar orbiters at altitudes of approximately 20 km and 40 km. Their maximum and minimum intensities, corresponding respectively to bright lobes and dark cusps on the lunar surface, align with the optical albedo patterns observed at Reiner Gamma. Our simulations show that the reflection area of solar wind particles above Reiner Gamma increases as the incident solar wind energy decreases. In the bright lobes, solar wind particle reflection exhibits a clear dependence on strong horizontal magnetic fields and dominant perpendicular energies. In contrast, reflection in the cusps is less definitive, being additionally governed by the interplay between relative perpendicular energy and magnetic configuration. We discuss the necessary conditions under which incident solar wind particles are absorbed at the surface or reflected above Reiner Gamma.

How to cite: Hong, Y., Kim, K.-H., Lee, J., Jin, H., and Baek, S.-M.: Interaction Between Solar Wind Particles and the Reiner Gamma Magnetic Anomaly: Observations and Test-Particle Simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8775, https://doi.org/10.5194/egusphere-egu26-8775, 2026.

EGU26-8778 | Orals | PS1.4

Tidally driven remelting of the Moon around 4.35 billion years ago 

Alessandro Morbidelli, Francis Nimmo, and Thorsten Kleine

The last giant impact on Earth is thought to have formed the Moon. The timing of this event can be determined by dating the different rocks assumed to have crystallized from the lunar magma ocean (LMO). This has led to a wide range of estimates for the age of the Moon between 4.35 and 4.51 billion years ago (Ga), depending on whether ages for lunar whole-rock samples or individual zircon grains are used. Here we argue that the frequent occurrence of approximately 4.35-Ga ages among lunar rocks and a spike in zircon ages at about the same time is indicative of a remelting event driven by the Moon's orbital evolution rather than the original crystallization of the LMO. We show that during passage through the Laplace plane transition, the Moon experienced sufficient tidal heating and melting to reset the formation ages of most lunar samples, while retaining an earlier frozen-in shape and rare, earlier-formed zircons. This paradigm reconciles existing discrepancies in estimates for the crystallization time of the LMO, and permits formation of the Moon within a few tens of million years of Solar System formation, consistent with dynamical models of terrestrial planet formation. Remelting of the Moon also explains the lower number of lunar impact basins than expected, and allows metal from planetesimals accreted to the Moon after its formation to be removed to the lunar core, explaining the apparent deficit of such materials in the Moon compared with Earth. We will also discuss how the Moon could have reached the Laplace Plane Transition so late during its tidal evolution.  

How to cite: Morbidelli, A., Nimmo, F., and Kleine, T.: Tidally driven remelting of the Moon around 4.35 billion years ago, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8778, https://doi.org/10.5194/egusphere-egu26-8778, 2026.

Lunar magnetic anomalies are abundant near the south pole, where several moderate-strength anomalies spatially overlap permanently shadowed regions. This environment provides a unique setting to assess how crustal magnetic fields and complex topography regulate plasma–surface interactions and, in turn, the stability and distribution of surface water ice.

A global fully kinetic electromagnetic particle-in-cell numerical model is used to simulate proton and electron surface fluxes near the south pole, averaged over a full lunar rotation. The simulations incorporate a regional crustal magnetic field model based on Kaguya and Lunar Prospector magnetometer measurements, together with high-resolution surface topography from the Lunar Reconnaissance Orbiter Laser Altimeter. This approach enables a self-consistent evaluation of how terrain and crustal magnetic fields jointly influence plasma access to the surface.

The simulations show that topography strongly structures the surface plasma environment, enhancing fluxes on crater walls while partially shielding crater floors. The inclusion of crustal magnetic fields further modulates plasma access, producing relatively modest proton and electron flux variations relative to simulations without magnetic anomalies.

Using the modelled fluxes, plasma-driven production, sputtering, and electron-stimulated desorption rates are evaluated alongside thermally driven sublimation. While the absolute balance depends on laboratory-derived yield assumptions, the results indicate that permanently shadowed regions consistently exhibit a positive net surface water ice balance rate, which closely coincides with inferred surface water ice exposures and highlights the importance of including realistic crustal magnetic fields and topography when assessing plasma-surface interactions and volatile evolution at the lunar poles.

How to cite: Deca, J., Hood, L., and Li, S.: The Role of Crustal Magnetic Anomalies and Topography in Shaping Lunar South Polar Water Ice, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8795, https://doi.org/10.5194/egusphere-egu26-8795, 2026.

EGU26-9059 | ECS | Posters on site | PS1.4

MEMS short-period chip-level seismometer for the next generation Lunar/Mars seismograph 

xingyu wei, chenhao du, qi wang, tiange wei, hao ouyang, qiu wang, and huafeng liu

China's Lunar Exploration Program aims to deploy advanced seismometers on the lunar surface for detecting and characterizing moonquakes, essential for understanding the Moon's internal structure. Compared to conventional seismic geophones, nano‑g‑resolution MEMS accelerometers offer superior sensitivity, compact size, and low power consumption—key attributes for space instrumentation. This paper presents a capacitive MEMS accelerometer designed for next‑generation lunar seismometry. Its sensing element consists of a movable silicon proof mass suspended by micromachined beams, with distributed capacitive electrodes detecting minute displacements.

Innovating beyond traditional parallel‑plate designs, a corrugated electrode structure reduces the second‑order nonlinear coefficient by half and the third‑order coefficient by two‑thirds, improving linearity without compromising footprint or sensitivity. Furthermore, the device incorporates an electrostatic negative stiffness mechanism, successfully reducing the intrinsic resonant frequency to 122 Hz. The decrease in resonant frequency improves the mechanical gain of the seismometer, thereby enhancing the instrument's sensitivity. The design also improves pull‑in stability, extending the operational measurement range.

Comprehensive experimental characterization validates the device's performance:

  • The fabricated short-period (SP) seismometer achieves a low noise floor of 7 ng/√Hz within the 0.5–3.5 Hz band, which is crucial for detecting faint seismic signals.
  • It exhibits a broad linear measurement range of ±34 mg and a high open-loop dynamic range of 134 dB. 
  • The device provides a –3 dB bandwidth of 180 Hz, supporting a wide frequency response.
  • Notably, its extreme miniaturization—with a MEMS die measuring only 5.2 mm × 6.5 mm and a mass under 20 milli-gram—makes it particularly suitable for weight-sensitive lunar missions.

This research has not only developed a high‑sensitivity MEMS sensor suitable for lunar seismology, but also holds significant potential for terrestrial geophysical applications such as precision seismic monitoring and oil‑gas exploration. The design provides a promising and robust technical pathway for the future development of high‑performance closed‑loop MEMS accelerometers.

Fig 1 The schematic view of the proposed MEMS accelerometer system

Fig 2 Noise performance of the proposed MEMS accelerometer in an open-loop configuration, in which the self-noise is the actual noise floor of the proposed device, with the elimination of the influence of Earth tremors.

How to cite: wei, X., du, C., wang, Q., wei, T., ouyang, H., wang, Q., and liu, H.: MEMS short-period chip-level seismometer for the next generation Lunar/Mars seismograph, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9059, https://doi.org/10.5194/egusphere-egu26-9059, 2026.

EGU26-11341 | ECS | Posters on site | PS1.4

Seismic, magnetic and gravity investigations of Lunar lava tubes: An Earth-analogue case study from Lanzarote island (Spain) 

Alessandro Ghirotto, Ilaria Barone, Francesco Santoro De Vico, Giacomo Melchiori, Andrea Zunino, Egidio Armadillo, Anna Mittelholz, Francesco Sauro, and Matteo Massironi

Lava tubes are subsurface volcanic conduits formed during effusive basaltic eruptions and are increasingly recognized as key targets for planetary exploration. On the Moon, orbital remote sensing imagery has revealed numerous collapse pits suggesting the presence of subsurface lava tube systems. These structures are of high scientific and exploration interest, as they may provide stable thermal environments, effective radiation shielding, and protection from impact hazards. However, the geophysical characterization of lunar lava tubes remains challenging, as current low-resolution orbital remote sensing techniques offer limited insight into their three-dimensional geometry, internal structure, spatial continuity and, in most cases, even their existence.

As future missions plan to deploy surface-based geophysical instruments, there is a growing need for robust and transferable integrated strategies to characterize subsurface lava tubes. Terrestrial lava tubes provide essential analogues for developing and validating such approaches, yet most existing studies rely on single geophysical techniques, limiting the completeness of subsurface interpretations.

Here, we present a comprehensive multi-method geophysical investigation of the lava tube “Cueva de Los Naturalistas” in the UNESCO Geopark of Lanzarote (Canary Islands), a well-established analogue for lunar volcanic terrains due to its basaltic composition, recent volcanic history and well-preserved lava tube system. We have conducted high-resolution, profile-based, active and passive seismic surveys coupled with magnetic and gravity investigations to image and characterize the subsurface geometry of the lava tube. Both passive and active seismic analyses reveal anomalous behaviour above the cavity, which strongly correlates with a negative magnetic and gravity anomaly. Joint 2D magnetic & gravity inverse modelling and 3D structural modal analysis of the roof of the lava tube allow us to constrain the tube’s location, dimensions and internal structure, highlighting the complementarity and suitability of the methods used and reducing ambiguities inherent in single-technique approaches.

Our results demonstrate the effectiveness of integrated seismic, magnetic and gravity surveying for lava tube characterization and provide a methodological strategy that can be adapted to future robotic and human missions on our natural satellite. This study contributes to closing a critical gap in our ability to assess subsurface cavities on the Moon and other planetary bodies.

How to cite: Ghirotto, A., Barone, I., Santoro De Vico, F., Melchiori, G., Zunino, A., Armadillo, E., Mittelholz, A., Sauro, F., and Massironi, M.: Seismic, magnetic and gravity investigations of Lunar lava tubes: An Earth-analogue case study from Lanzarote island (Spain), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11341, https://doi.org/10.5194/egusphere-egu26-11341, 2026.

EGU26-11531 | Posters on site | PS1.4

LunarLeaper - Exploring Lunar Lava Tubes  

Simon C. Stähler, Anna Mittelholz, Valentin T. Bickel, Aurélie Cocheril, Adrian Fuhrer, Alessandro Ghirotto, Matthias Grott, Svein-Erik Hamran, Natanael Hirzel, Jonas Isler, Ozgur Karatekin, Yara Luginbühl, and Birgit Ritter

 

LunarLeaper is a robotic mission concept aimed at advancing our understanding of the Moon’s subsurface structure and geological evolution through the exploration of volcanic pits—steep-walled collapse features on the lunar surface. Orbital observations indicate that some of these pits may provide access to extensive subsurface lava tube systems. However, such interpretations are limited by spatial resolution and viewing geometry, and only an in-situ surface mission can unambiguously confirm and characterize the relationship between pits and underlying caves. We propose the use of a legged robotic platform to deploy geophysical instrumentation to the rim of a lunar pit on the near side of the Moon. From this vantage point, the mission will confirm the presence of a lava tube, constrain its geometry, and employ imaging and spectrometric measurements to reconstruct the volcanic history of the pit and its surrounding terrain.

The baseline payload for LunarLeaper consists of a camera system, a ground-penetrating radar, a gravimeter, and a spectrometer. We report the current status of payload accommodation on the robotic platform:

  • The camera requirements for the mission can be met by an COTS camera system previously used as engineering cameras for ESA spacecraft, such as BepiColombo.
  • We have developed a compact, PCB-based antenna system for the ground-penetrating radar that can be fully integrated beneath the robot body.
  • Forward modelling of the expected gravimetric signal, combined with a preliminary noise budget that accounts for instrument tilt, shows that the sensitivity of the HERA-heritage gravimeter exceeds mission requirements by approximately an order of magnitude.
  • Measurements with the Fabry-Perot spectrometer have been demonstrated against several mineralogical compositions.
  • A preliminary concept of operations demonstrates that payload operation and data acquisition are compatible with overall mission constraints, specifically the mission duration of less than one lunar day.

Together, these results demonstrate that the combined geophysical and imaging payload suite can be accommodated on a small robotic platform, as currently being developed by the Robotic Systems Lab at ETH Zürich.

How to cite: Stähler, S. C., Mittelholz, A., Bickel, V. T., Cocheril, A., Fuhrer, A., Ghirotto, A., Grott, M., Hamran, S.-E., Hirzel, N., Isler, J., Karatekin, O., Luginbühl, Y., and Ritter, B.: LunarLeaper - Exploring Lunar Lava Tubes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11531, https://doi.org/10.5194/egusphere-egu26-11531, 2026.

EGU26-12566 | Posters on site | PS1.4

Observations of the 2025 Geminid Lunar Impact Flashes with TILT 

Daniel Sheward, Marco Delbo, Piere-Yves Froissart, Christelle Saliby, Jean-Pierre Rivet, Philippe Lognonné, and Chrysa Avdellidou

During the 2025 Geminids, which peaked between 2025-12-13 and 2025-12-14, the Moon was between 30-40% illuminated, with the radiant of the Geminid meteoroid stream on the unilluminated hemisphere of the Moon. This orbital geometry, coupled with the favourable observation conditions, prompted a global campaign to observe Lunar Impact Flashes (LIFs). As part of the commissioning phase of the TILT instrument (a dual 40 cm Newtonian telescope system based in Calern, France, built for coordinated LIF observations alongside lunar-based seismometers, see abstract EGU26-7444 for more detail), we took part in this observation campaign.

TILT operated for the totality of the observable period over these two nights, obtaining a total of 8.5 hours of LIF observations. Five hours of observation were performed on 2025-12-13, using two visible cameras (one ASI183MM, and one ASI174MM), and a further three and a half hours were performed on 2025-12-14, using one visible camera (ASI183MM) and one short-wave infrared camera (Ninox 640SU). From this data, we detected 56 events which could not be immediately rejected as false positives and were so far able to confirm nine of these events as true LIFs, through the LIF lasting more than one frame (4 events), and by observing the flashes in multiple simultaneous observations (5 events). While we are unable to confirm with certainty that these events were belonging to the Geminids (due to the constant presence of the sporadic background population), all the confirmed LIFs exhibited impact geometry compatible with the Geminid meteoroid stream. After performing photometric calibration of these events using stars observed at a similar airmass throughout the observations, we found that the confirmed events have magnitudes ranging between +7.5 and +10.4. These impacts are estimated to have formed craters ranging between 0.7 m and 1.7 m rim-to-rim diameter.

Preliminary results suggest a rate of impacts of 1.1 hr-1 for confirmed events, and 6.6 hr-1 events for all events. For the purposes of multi-messenger observations with lunar seismometers, confirmation of the events can be performed using the seismic signal of the impact, and therefore confirming the impacts occurrence based solely on LIF observations is not required. Hence, this observation campaign has demonstrated the importance of observing during high impact-rate streams, such as the Geminids, for the future operations of TILT.

How to cite: Sheward, D., Delbo, M., Froissart, P.-Y., Saliby, C., Rivet, J.-P., Lognonné, P., and Avdellidou, C.: Observations of the 2025 Geminid Lunar Impact Flashes with TILT, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12566, https://doi.org/10.5194/egusphere-egu26-12566, 2026.

EGU26-12596 | Orals | PS1.4

Magnetic Anomalies Near the Lunar South Pole and Their Consequences  

Lon Hood, Jan Deca, Shuai Li, and Daniel Moriarty

We report improved mapping of crustal magnetic anomalies near the lunar poles using a combination of Lunar Prospector and Kaguya orbital magnetometer data.  In agreement with previous results, a concentration of moderately strong magnetic anomalies is centered approximately on the south polar region.  In contrast, only a single verified anomaly is present in the north polar region.  Published analyses of Kaguya spectral profiler and LOLA albedo data have shown that an area of relatively low optical maturity and high surface albedo is present in the south polar region whereas the north polar region is mostly optically mature. Comparing our magnetic field maps to published albedo maps (D. Moriarty and N. Petro, JGR, 2024), possible curvilinear albedo markings (“swirls”) of the Reiner Gamma class are present where the strongest anomalies near the south pole are found. In the north polar region, a single albedo anomaly is present just poleward of the single magnetic anomaly. In view of previous work showing that solar wind ion deflection associated with crustal magnetic fields can lead to surface optical immaturity, higher surface albedo, and swirl formation, the empirical evidence reported here supports the hypothesis that the magnetic anomalies near the south pole are capable of significant solar wind ion flux reductions. 

Previous analyses of Moon Mineralogy Mapper (M3) data have also found that more inferred water ice exposures are present near the south pole than near the north pole (S. Li et al., PNAS, 2018).  We have previously reported particle-in-cell simulations of the surface plasma flux and water ice lifetimes against solar wind ion sputtering in this region, taking into account crustal magnetic fields as well as topography (J. Deca et al., 2025 LPSC; 2026 LPSC).  These simulations demonstrate a correlation between areas of long sputtering lifetimes and areas with more numerous water ice exposures.  Further simulations using the improved crustal field maps are in progress and will be presented at the meeting.

How to cite: Hood, L., Deca, J., Li, S., and Moriarty, D.: Magnetic Anomalies Near the Lunar South Pole and Their Consequences , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12596, https://doi.org/10.5194/egusphere-egu26-12596, 2026.

EGU26-13113 | Posters on site | PS1.4

PGEs and Re-Os in CE-5 Lunar Soil: Implications for Late Accretion to the Moon 

Guiqin Wang, Yuling Zeng, Yangting Lin, and Jifeng Xu

The late accretion of exotic materials is significant in the study of the formation and evolution of the Earth and the Moon. The importance of platinum-group elements (PGEs) in tracking the late accretion stages of planetary formation has long been recognized. In previous studies, estimates of the flux of exotic materials added to the Moon have primarily been based on measurements of siderophile element concentrations in lunar regolith samples returned by the Apollo or Lunar missions. However, due to the analytical limitations at that time, only a few individual siderophile elements, such as Ni, Ir, Ge, Re, and Au, could be quantified. Among these elements, Ni is moderately siderophile, while Ge is moderately volatile, which means neither is the most ideal tracer for identifying the exotic materials in the moon. Advances in analytical techniques have significantly enhanced both the precision and accuracy of measurements for PGEs and Os isotopes. High-precision analytical techniques have established characteristic of PGEs patterns and Os isotope ratios in different meteorite types by ICPMS and TIMS. However, to date, no detailed study has been conducted on PGEs and Os isotopes in mature lunar soil.

The CE-5 lunar soil (CE-5LS) collection site is located in an area far from the Apollo and Luna mission regions, and previous studies have confirmed that the surface basalts in the CE-5 sampling area are more than 1 billion years younger than those in the Apollo and Lunar mission regions[1, 2]. This implies that the exotic material flux and composition within the CE-5LS may differ significantly from those in the Apollo lunar soil.

In this study, 1100 mg of CE-5LS samples were magnetically separated. And PGEs and Os isotopes were analyzed on the magnetic and non-magnetic fractions, respectively. The results indicate that the influx of exotic material at the CE-5 landing site amounted to approximately 0.8%, markedly lower than estimates based on the accumulation of exotic material in Apollo soil samples (1%–5%)[3-7]. Given that the accumulation of extraterrestrial material on the Moon correlates positively with the Moon's age, this conclusion is reasonable. The PGE patterns and Os isotope ratios in CE-5LS are consistent with those analysed in chondrites. Consequently, the exotic material accrated onto the Moon is predominantly chondrites.

 

Acknowledgment

The authors had the great honour of applying for and receiving approval to carry out studies on the CE-5 lunar samples allocated by the CNSA. This work was financially supported by the National Key Research and Development Project of China (2020YFA0714804).

 

Reference

[1] Che X. C., et al. (2021). Science 374:887.

[2] Li Q. L., et al. (2021). Nature 600:54.

[3] Ganapathy R., et al. (1970). Geochimica et Cosmochimica Acta Supplement 1:1117.

[4] Baedecker P. A., et al. (1974). Lunar and Planetary Science Conference Proceedings 2:1625-1643.

[5] Laul J. C., et al. (1974). Lunar and Planetary Science Conference Proceedings 2:1047-1066.

[6] Boynton W. V., et al. (1975). Lunar and Planetary Science Conference Proceedings 2:2241-2259.

[7] Higuchi H. and Morgan J. W. (1975). Lunar and Planetary Science Conference Proceedings 2:1625-1651.

How to cite: Wang, G., Zeng, Y., Lin, Y., and Xu, J.: PGEs and Re-Os in CE-5 Lunar Soil: Implications for Late Accretion to the Moon, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13113, https://doi.org/10.5194/egusphere-egu26-13113, 2026.

EGU26-14643 | ECS | Orals | PS1.4

Biomining of Lunar-Relevant Materials under Simulated Lunar Gravity on the International Space Station 

Andrew Acciardo, Rosa Santomartino, Charles Cockell, Cara Magnabosco, Henner Busemann, Ingo Leya, Cyprien Verseux, and Audrey Vorburger

With near-future manned space exploration expanding beyond low Earth orbit out toward the Moon and beyond, there is a critical need to understand how a sustained human lunar presence can be supported through in-situ resource utilization (ISRU), as transporting supplies to the lunar surface remains technically challenging and costly(Y. Gumulya et al., Minerals Engineering, 2022; R. Santomartino et al., Nature Communications, 2023). Biomining, a terrestrial biotechnology that employs microorganisms to mobilize useful elements from rock, represents a promising approach for space-based ISRU. Recent biomining experiments aboard the International Space Station (ISS), including BioRock using Martian rock analogs and BioAsteroid using meteoritic material, have demonstrated that microbial mobilization of economically and ISRU-relevant elements is feasible in space(C. S. Cockell et al., Nature Communications, 2020; R. Santomartino et al., in review). However, biomining of lunar(-like) material, particularly under lunar-like gravitational conditions, has not yet been explored. For lunar-specific biomining, heterotrophic organisms might be more suitable than chemolithotroph ones, due to their capacity to bioleach silicon-rich minerals. The use of cyanobacterial biomass as a reusable “nutrient cartridge” to support their organics requirement in space represents a key but untested component of closed-loop ISRU systems (R. Santomartino et al., Nature Communications, 2023; C. Verseux et al., Frontiers in Microbiology, 2021).

Here, we propose an ISS experiment to investigate biomining of lunar KREEP-like material under multiple gravity regimes. The primary objectives are to (1) quantify biomining performance on lunar(-like) substrates under simulated lunar gravity, (2) compare biomining efficiency across multiple gravitational conditions, (3) test whether cyanobacterial biomass enhances biomining performance, and (4) demonstrate metabolic coupling between autotrophic biomass and heterotrophic microorganisms under lunar-relevant gravity. The experiment will employ flight-proven bioreactor hardware containing Sphingomonas desiccabilis, a microorganism previously shown to biomine rock under spaceflight conditions, partially supplied with stable isotope-labelled biomass derived from Anabaena cylindrica. Biomass from this cyanobacterium, which is being studied for its ability to grow from resources available on the Moon or Mars, has previously been demonstrated to support the heterotrophic growth of other organisms.

Incubations will be conducted within the existing KUBIK facility aboard the ISS, which provides controlled temperature conditions and simulated gravity environments. Following sample return to Earth, a combination of microbiological, chemical, isotopic, and geological analyses will be performed to assess microbial activity, element mobilization, and metabolic coupling. Multiple gravity regimes, along with Earth-based ground controls, will allow direct evaluation of gravitational effects on biomining efficiency and microbial physiology.

We expect to observe measurable mobilization of rare earth and other ISRU-relevant elements from the mineral substrate, as well as isotopic signatures indicating utilization of cyanobacterial biomass by S. desiccabilis. Differences in metal-leaching efficiency and microbial responses across gravity conditions are anticipated. This experiment will provide the first proof-of-concept demonstration of biologically mediated loop-closure relevant to lunar ISRU, informing future strategies for sustainable lunar exploration and advancing our understanding of microbe-mineral interactions beyond Earth.

How to cite: Acciardo, A., Santomartino, R., Cockell, C., Magnabosco, C., Busemann, H., Leya, I., Verseux, C., and Vorburger, A.: Biomining of Lunar-Relevant Materials under Simulated Lunar Gravity on the International Space Station, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14643, https://doi.org/10.5194/egusphere-egu26-14643, 2026.

EGU26-15457 | ECS | Orals | PS1.4

Global Sub-Decameter-Scale Roughness of the Moon’s Surface 

Hephzibah Christopher and Indujaa Ganesh

Surface roughness is an effective parameter for mapping geomorphological units and for quantifying the topographic evolution of the Moon’s surface, as it records the effects of impact cratering, regolith processes, and geological modification [1,2]. It highlights surface features that are often difficult to detect in optical images and conventional digital elevation models (DEMs). Additionally, roughness at small spatial scales is valuable for assessing landing site hazards and for interpreting radar remote sensing observations. However, existing global lunar roughness maps are largely limited to ~10 m and longer baselines, thereby hindering spatially detailed studies of surface geology.

We present novel estimates of global surface roughness for the Moon at ~5 m length scales, determined from Lunar Orbiter Laser Altimeter (LOLA) echo pulse width measurements. In addition to measuring surface elevations from time-of-flight ranging, LOLA recorded the width of reflected laser pulses, which is sensitive to vertical variations within the illuminated footprint of ~5 m diameter. LOLA pulses reflected from the Moon’s surface are broadened relative to the transmitted pulses due to surface slopes and small-scale roughness. We determine small-scale roughness from the amount of pulse broadening, after correcting for factors such as beam divergence and curvature, observation geometry, the temporal decline in transmitted power, and receiver misalignment during polar and nightside crossings [3,4].  

Roughness at sub-decameter scales (~5 m) reveals signatures of recent and ongoing surface processes on the Moon. The youngest impact craters, formed in the Copernican period, are distinctly rough, with interiors rougher than their ejecta blankets. The high-albedo swirl Reiner Gamma also appears unusually rough at these scales, despite lacking evident topographic expression, with on-swirl areas rougher than off-swirl. In the polar regions, permanently shadowed regions are smoother than nearby sunlit areas even on gentle slopes (<20°), suggesting potential for volatile preservation [5]. Among Artemis III candidate sites in the south pole, the Mons Mouton Plateau and Haworth are the smoothest and most favorable sites for rover navigation and extravehicular activities. Thus, our small-scale roughness map complements existing longer-baseline roughness products, captures topographic variability at spatial scales most relevant to upcoming surface missions, and provides new insight into recent modification of the lunar surface.

 

References: [1] Shepard M. K. et al. (2001) JGR, 106, 32777–32795. [2] Kreslavsky M. et al. (2013) Icarus, 226, 52-66. [3] Gardner C. S. (1992) IEEE Trans. Geosci. Remote Sens., 30, 1061–1072. [4] Neumann G. A. et al. (2003) GRL, 30(11). [5] Magaña L. O. et al. (2024) Planet. Sci. J., 5(2), 30.

How to cite: Christopher, H. and Ganesh, I.: Global Sub-Decameter-Scale Roughness of the Moon’s Surface, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15457, https://doi.org/10.5194/egusphere-egu26-15457, 2026.

EGU26-15644 | ECS | Posters on site | PS1.4

Subscale Experiment for Investigating Lunar Magnetospheres 

Patrick Rae, Arvindh Sharma, and Justin Little

Lunar magnetic anomalies (LMAs) show a curious ability to reflect the high velocity ions (~400 km/s) of the solar wind, an effect of interest for manned missions. As it stands, current work in this area has focused primarily on simulation efforts supported by spacecraft data. There is a pressing need to better understand the structure of the miniature-magnetosphere system over a wide range of solar wind parameters if human missions come to rely on this shielding effect. To better target the fundamental physics of the miniature-magnetosphere, we propose an approach using a subscale experiment.

To investigate the basic physics and scaling parameters of the miniature-magnetosphere in a controlled setting, we constructed an experiment capable of recreating this plasma interaction at the laboratory scale. Specifically, we wish to investigate the magnitude, location, and thickness of the repelling electric field and how these parameters are influenced by the simulated solar wind.

A picture of the experiment in operation can be seen in [FIG. 1]. The simulated solar wind is created using an RF discharge and a DC voltage across two molybdenum grids. The resulting ion beam is neutralized by a hollow cathode mounted in the test chamber. The solar wind impacts the experiment assembly consisting of a Garolite (G-10) sheet acting as the lunar surface, a neodymium magnet beneath the surface mimicking the LMA, and a 3-axis translation stage actuating the probes. The entire platform can rotate ≤30° to simulate different solar wind incidence angles.

Emissive and Langmuir probes were chosen as diagnostics. The first measures plasma potential while operating in half-wave AC heating mode. The second measures ion density, electron temperature, and plasma potential. Initial results only report the ion saturation current which scales linearly with density and the root of the electron temperature. The  scaling is important because spacecraft data shows elevated electron temperatures produced in the mini-magnetosphere.

The experiment is supported by 3D particle in cell (PIC) simulations to bridge the gap between experimental and lunar length scales. The two work in tandem to inform one another to better isolate the driving principles of the system.

Initial results from the emissive probe [FIG. 2] show a peak plasma potential of ~200 V directly above the magnet. This value monotonically decreases with distance to the magnet which is consistent with an outward electric field being established. The map of ion saturation current [FIG. 3] is not fully complete at the time of submission but does further corroborate the formation of an ion cavity surrounded by a higher density barrier region.

Visual observations of the plasma show an asymmetry across the magnetic axis that is consistent with the 3D PIC model. This “stretching” of the magnetosphere in one direction is consistent with an  drift.

Complete 3-D maps of the density, potential, and temperature of the plasma will be ready by the conference date. A parametric investigation of various solar wind input conditions will also be conducted.

How to cite: Rae, P., Sharma, A., and Little, J.: Subscale Experiment for Investigating Lunar Magnetospheres, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15644, https://doi.org/10.5194/egusphere-egu26-15644, 2026.

EGU26-15867 | Orals | PS1.4

South Pole-Aitken basin sample Return and eXploration (SPARX) Science Definition Team Report: Findings and Recommendations for a Future Lunar Mission 

Lauren Jozwiak and the South Pole Aitken basin sample Return and eXploration (SPARX) Science Definition Team

Sample return from the Moon’s South Pole-Aitken Basin (SPA) has long been recognized as a high priority destination for lunar science, appearing as a recommended medium-class NASA mission in multiple United States National Academies of Sciences Planetary Science decadal surveys. The primacy of the site arises from the unique combination of its size, antiquity, and location on the lunar farside. The South Pole-Aitken basin presents the ideal target destination to test nearly 60 years of lunar science hypotheses. Despite the recognized importance of the science, mission proposals for sample return have previously been hampered by a combination of costs and technology. During the development of the 2023-2032 Origins, Worlds, and Life (OWL) decadal survey, a mission concept named “Endurance” demonstrated the feasibility of a long-duration, long-traverse mission that could accomplish the majority of defined priority lunar science investigations at a cost cap that was commensurate with New Frontiers scale missions. This mission concept leveraged new developments in rover technology, autonomous systems development, and concepts of operations developed by the Intrepid Pre-decadal Mission Concept Study, in conjunction with the advent of technological advances in the commercial exploration marketplace. Using the Endurance point design, the OWL advocated for the development of an SPA Sample Return mission as the highest priority mission for the Lunar Discovery and Exploration Program (LDEP). In response to this recommendation, NASA convened the South Pole Aitken basin sample Return and eXploration (SPARX) Science Definition Team (SDT) to provide analysis on prioritized science objectives and implementation architectures for a South Pole-Aitken Basin sample return mission.

The SPARX SDT report will be released to the community in Spring 2026, following review by NASA. The report will include descriptions of prioritized science goals and objectives and the associated requirements for both in-situ and terrestrial laboratory measurements. The report will provide a description of a baseline implementation architecture that demonstrates a notional traverse and mission architecture for accomplishing all of the listed science objectives. Additionally, the report will include a discussion of multiple mission implementation profiles, with recommendations for their future selection criteria. Finally, the report will contain a discussion of future technologic and programmatic factors that could affect the future implementation of the mission, including the role of astronauts, commercial exploration, and international participation. This presentation will provide an overview of the newly released SPARX report, focusing on the overarching recommendations for implementation architectures, measurement requirements, and high-priority items for the next phases of mission development.

How to cite: Jozwiak, L. and the South Pole Aitken basin sample Return and eXploration (SPARX) Science Definition Team: South Pole-Aitken basin sample Return and eXploration (SPARX) Science Definition Team Report: Findings and Recommendations for a Future Lunar Mission, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15867, https://doi.org/10.5194/egusphere-egu26-15867, 2026.

EGU26-16079 | ECS | Orals | PS1.4

Particle-In-Cell and Experimental Study of Lunar Mini-Magnetospheres for Power Extraction 

Arvindh Sharma, Patrick Rae, Vignesh Krishna Kumar, Jan Deca, and Justin Little

Lunar magnetic anomalies (LMAs) are small regions (on the order of 100 km) of crustal magnetic fields on the lunar surface with field strengths of about 100 nT [1, 2]. Spacecraft measurements and numerical modeling of the interaction between the solar wind and the LMAs predict the formation of mini-magnetospheres [3], where the field strength magnetizes electrons but not ions. The separation between the electrons tied to the field lines and the less restrained ions produces strong electric fields (≈ 0.150 V m−1) near the lunar surface [1]. At SPACE Laboratory, we are studying if this polarization electric field and the solar wind particle flux can be used for power extraction on the lunar surface using 3D particle-in-cell (PIC) modeling [4] and a subscale experiment. The figure shows key aspects employed to simulate mini-magnetosphere physics in the PIC code (left) and the experiment (right): (1) a plasma representing the solar wind, (2) a magnetic dipole field representing the LMA, (3) the lunar surface plane, (4) a current emitting cathode that enhances and allows power draw into an external load, and (5) an anode where electron precipitation balances the load current. The simulation imposes sheath electric field conditions at the electrodes [5, 6] to model the interaction with the plasma.

This work presents results from a study of mini-magnetosphere structure under various solar wind conditions, such as varying incidence angle, density, and speed, and discusses how the changing plasma dynamics would affect power extraction. Results show that net positive power in the sub-kilowatt range can be extracted from the mini-magnetosphere under favorable conditions with the injection of an electron current from the cathode and the collection of sufficient charged particles at the anode. PIC simulations show that the stability of the power generation scheme depends on the stability of the mini-magnetosphere structure, which is sensitive to the cathode electron injection. Moreover, the solar wind incidence angle is found to be a major factor in determining the power that could be generated with fixed electrodes since the mini-magnetosphere structure stretches in the direction of the wind. The subscale experiment corroborates many of the physical phenomena predicted by the simulations, lending credence to the findings. Based on the physical insights, we propose engineering solutions that could enable this technology to provide power for lunar exploration missions.

References: [1] Deca J. et al. In: Journal of Geophysical Research: Space Physics 120.8 (2015), pp. 6443–6463. [2] Bamford R. A. et al. In: The Astrophysical Journal 830.2 (2016), p. 146. [3] Deca J. et al. In: Physical Review Letters 112.15 (2014), p. 151102. [4] Markidis S. et al. In: Mathematics and Computers in Simulation 80.7 (2010), pp. 1509–1519. [5] Skolar C. R. et al. In: Physics of Plasmas 30.1 (2023), p. 012504. [6] Baalrud S. D. et al. In: Plasma Sources Science and Technology 29.5 (2020), p. 053001.

How to cite: Sharma, A., Rae, P., Krishna Kumar, V., Deca, J., and Little, J.: Particle-In-Cell and Experimental Study of Lunar Mini-Magnetospheres for Power Extraction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16079, https://doi.org/10.5194/egusphere-egu26-16079, 2026.

Apollo seismic data have greatly advanced our understanding of the Moon’s internal structure and seismic activity, but they also contain many glitches produced by the harsh lunar environment. For example, around lunar sunrise and sunset, hundreds of anomalous signals are typically recorded within a few hours. Characterizing the waveforms, distribution patterns, and causes of these glitches is essential, as it can provide important references for reducing the occurrence of anomalous signals during the observation and suppressing their interference during the analysis, thereby offering useful guidance for the implementation and data processing of seismic observations in upcoming lunar missions. In this study, we combined deep learning with template matching to detect and catalog acceleration-related glitches in the Apollo seismic records. The resulting catalogs reveal clear temporal patterns that correlate with lunar diurnal and seasonal cycles. Glitches around lunar sunrise and sunset are likely driven by rapid temperature changes, while daytime glitches are linked to shading by nearby objects or to lunar eclipses. Notably, we also found eclipse-related glitches. Because the instrument temperature changes induced by lunar eclipses are more abrupt than those at sunrise and sunset, this issue should be taken into account in future lunar seismic observations. We also identify elliptically polarized glitches, which differ from the predominantly linear polarization reported for Martian glitches and merit further investigation. The glitch catalogs show substantially fewer glitches during the lunar night than during the day, offering practical guidance for optimizing observation windows. In addition, station-to-station differences in daytime glitch patterns underscore the strong influence of site location and instrument deployment on data quality, which is an important consideration for future lunar missions. In summary, this work compiles acceleration-related glitch catalogs from Apollo seismic data, clarifies how the lunar environment affects seismic observations, and provides useful references for optimizing observing strategies and instrument deployment in upcoming missions.

How to cite: Liu, X., Xiao, Z., and Li, J.: Acceleration-Related Glitch Patterns in Apollo Seismic Data and Implications for Future Lunar Seismic Observation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16218, https://doi.org/10.5194/egusphere-egu26-16218, 2026.

EGU26-17808 | ECS | Posters on site | PS1.4

Consequences of a volatile-rich bulk silicate Moon for its core and transient atmosphere 

Cordula P. Haupt, Francis M. McCubbin, and Fabrice Gaillard

It is widely accepted that the Moon lost most of its volatiles during formation by a catastrophic impact and subsequent accretion from a hot debris disk.[1] However, analyses of primitive lunar samples (e.g., olivine-hosted melt inclusions) indicate that portions of the lunar silicate mantle (bulk silicate Moon; BSM) may retain significant amounts of volatiles.[2] A recent compilation [3] provides best estimates for BSM volatile abundances, including S, H, O, and C, with hydrogen showing the greatest variability. In parallel, remote sensing data reveal water ice deposits in permanently shadowed polar regions of the Moon, implying the presence of water reservoirs today.[4]

Despite these observations, the implications of a volatile-rich BSM for the Moon’s differentiation and resulting reservoirs (core-mantle-atmosphere) remain poorly explored. Here, we apply a state-of-the-art differentiation model developed in our lab [5] inspired by recent work [6, 7] that tracks volatile partitioning using experimental volatile solubility laws for silicate melt, metal, and gas. The model is benchmarked against proposed BSM volatile inventories.[3] We assess the impact of a range of mantle volatile contents on the composition of the Fe-dominated lunar core. We deduce plausible volatile abundances (in wt% of the core) of S = 0.4–1.1, H < 10-4; O ≈ 0.1, and C = 0.05–0.16. We further evaluate composition and mass of an atmosphere generated during lunar magma ocean degassing. Such an atmosphere is CO and H2-dominated, with total pressures of 0.5–6 bar, PH2O/PH2 ≈ 0.05 and PCO/PCO2 = 63.7–64.6. Our results provide new constraints on volatile redistribution during lunar differentiation and support a magmatic contribution to the formation of lunar polar ice.

 

1 Kato et al. 2015 Nature Communications (6) 7617, 2 Saal et al. 2008 Nature (454) 192-195, 3 McCubbin et al. 2023 Reviews in Mineralogy and Petrology (89) 729-786, 4 Li et al. 2018 PNAS (115) 8907-8912, 5 https://calcul-isto.cnrs-orleans.fr/apps/magworld_III/, 6 Gaillard et al., 2021 Space Science Reviews (217), 7 Gaillard et al., 2022 Earth and Planetary Science Letters (577) 117255

How to cite: Haupt, C. P., McCubbin, F. M., and Gaillard, F.: Consequences of a volatile-rich bulk silicate Moon for its core and transient atmosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17808, https://doi.org/10.5194/egusphere-egu26-17808, 2026.

EGU26-18513 | Posters on site | PS1.4

Design and Development of an All-Sky Electrostatic Analyzer 

Tzu-Fang Chang, Chih-Yu Chiang, Yu-Rong Cheng, Tzu-En Yen, Sheng-Cheng Tsai, Cheng-Tien Chen, Ping-Ju Liu, and Yung-Tsung Cheng

The All-Sky Electrostatic Analyzer (A-ESA) is a scientific payload designed for installation on a lunar rover, which will observe variations of the plasma environment on the Moon. Since the launch of the science payload project, the team from National Cheng Kung University (NCKU) have successfully completed the PDR, CDR, TRR, and PAR reviews. By the end of 2024, the team from NCKU delivered the A-ESA to the Taiwan Space Agency (TASA). In early 2025, the A-ESA was sent to the Lunar Outpost for integration testing. A-ESA consists of an electrostatic analyzer on top, while an MCP assembly, power supply units, and electronics are located underneath. A-ESA features entrance scanning deflectors and inner scanning deflectors. The entrance of A-ESA is electrically scanned within approximately 90° in the vertical direction, resulting in a hemispherical field of view (FOV). When A-ESA operates in observation mode, it divides the collection of scientific data into 8 sections horizontally and 6 sections vertically. By sweeping high voltage, it generates 16 different energy levels. As a result, A-ESA can measure the plasma distribution function and the energy of charged particles in a hemispherical space on the lunar surface.

How to cite: Chang, T.-F., Chiang, C.-Y., Cheng, Y.-R., Yen, T.-E., Tsai, S.-C., Chen, C.-T., Liu, P.-J., and Cheng, Y.-T.: Design and Development of an All-Sky Electrostatic Analyzer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18513, https://doi.org/10.5194/egusphere-egu26-18513, 2026.

EGU26-18687 | ECS | Posters on site | PS1.4

Projected Environmental Impacts of Helium-3 Mining on the Lunar Surface 

Miles Timpe

As commercial and governmental interest in lunar resource utilization intensifies, helium-3 mining has re-emerged as a frequently cited motivation for sustained human and robotic activity on the Moon. Helium-3 is a rare isotope with applications in neutron detection (e.g., national security, medical imaging), quantum computing, and as a proposed fuel for advanced nuclear fusion concepts. However, the expected low concentrations of helium-3 in the lunar regolith raises significant questions regarding the environmental consequences of its extraction at any meaningful scale.

Analyses of samples returned by the Apollo and Chang’e missions indicate that helium-3 is present in the lunar regolith at concentrations of only a few parts per billion. Because it is implanted by the solar wind, helium-3 is concentrated primarily in the uppermost centimeters of the regolith, with abundances decreasing exponentially with depth. As a result, any plausible extraction architecture must process extremely large volumes of regolith to recover modest quantities of helium-3. Proposed concepts range from shallow surface scraping to excavation of regolith to depths of up to several meters, implying disturbance over vast surface areas.

In this work, I model the spatial extent of helium-3 mining required to meet a range of plausible future helium-3 demand scenarios. These scenarios encompass continued use in neutron detection technologies, emerging quantum computing architectures, and speculative deuterium–helium-3 (D-He3) fusion energy systems.

The results demonstrate that while neutron detection and other low-demand applications require comparatively limited surface disturbance, demand from quantum computing already implies mining areas extending over tens to hundreds of square kilometers. Although substantially smaller than fusion-driven scenarios—which imply surface areas several orders of magnitude larger—quantum computing demand alone would generate surface disturbances which could be detectable by Earth-based observers using mass-market telescopes, binoculars, or consumer-grade imaging systems. Fusion demand would therefore overwhelmingly dominate the ultimate spatial footprint of helium-3 extraction, but non-fusion applications cannot be considered environmentally negligible.

Beyond the scale of disturbance, the environmental consequences of proposed extraction methods remain poorly constrained. Many concepts rely on mechanical agitation, excavation, or high-temperature processing of regolith, all of which may alter grain size distributions, maturity, and optical properties of the lunar surface. If mining activities produce a persistent change in surface albedo or spectral reflectance, large helium-3 mining fields could become visible from Earth. Under fusion-driven demand scenarios, such alterations could plausibly render mining regions visible to the naked eye, raising scientific, cultural, and policy concerns.

Given the extremely slow rates of natural weathering and regolith gardening on the Moon, any anthropogenic surface modification associated with helium-3 mining would persist for timescales well beyond humans. I conclude that targeted laboratory experiments, modeling studies, in situ measurements, and independent monitoring of proposed helium-3 extraction attempts are urgently needed to constrain the environmental impacts of helium-3 mining. Until such impacts are better understood, a precautionary approach to large-scale lunar helium-3 mining is warranted.

How to cite: Timpe, M.: Projected Environmental Impacts of Helium-3 Mining on the Lunar Surface, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18687, https://doi.org/10.5194/egusphere-egu26-18687, 2026.

EGU26-19727 | Posters on site | PS1.4

Interdisciplinary exploration science enabled by lunar landers: AstroLEAP sciences 

Yoshifumi Futaana, Iannis Dandouras, Patrick Fröhlich, Maria Genzer, Benjamin Grison, Antti Kestilä, Angèle Pontoni, Sylvain Ranvier, Jan Leo Loewe, Leo Nyman, Audrey Vorburger, Laurentiu Nicolae Daniel, Philipp Hager, Francesca McDonald, and Fabrice Cipriani and the AstroLEAP Facility Definition Team and AstroLEAP Study Team

The Moon is a unique and accessible target that hosts a distinctive space environment. It provides an opportunity to investigate fundamental physics associated with interactions with the undisturbed solar wind, magnetosheath, and magnetosphere. During disturbed space weather events, the lunar environment is influenced by hot plasma within the coronal mass ejections or high-energy particles such as solar energetic particles or cosmic rays. In the absence of an intrinsic magnetic field and a collisional atmosphere, the solar wind directly impacts the lunar surface, resulting in a plasma–regolith interaction, the physics of which remains poorly explored.

 

The interaction also sputters surface volatiles, producing the exosphere, a fragile gaseous environment surrounding the Moon. Space plasma may also contribute to the formation of surficial water, which can subsequently be released into the exosphere or space by meteoroid impacts. However, direct observational evidence for the production, circulation, and accumulation of such species remains highly limited. In addition, the Moon has localized magnetic anomalies that modify the incident plasma flow and, consequently, the near-surface environment. These disturbances are known as mini-magnetospheres, the smallest magnetospheres known. Local disturbances from environmental changes (electromagnetic fields, illumination, and their temporal variations) can induce significant dust lofting. Lunar dust poses a major hazard to human and robotic explorers. It is adhesive, potentially toxic, and easily mobilized. Dust particles can easily infiltrate electronics systems and spacesuits, and are significantly influenced by near-surface electric and magnetic fields. Furthermore, since the beginning of the space age, the lunar environment has been increasingly altered by human activities. Planned or ongoing exploration is expected to accelerate this anthropogenic modification. Quantifying the lunar environment is therefore urgently required to distinguish between its (near-)pristine state and its altered conditions on a decadal time scale.

 

In this presentation, we provide an overview of the multidomain physical processes—both natural and anthropogenic— that occur at the lunar surface in the context of future lunar surface missions.  We identify key open scientific questions concerning the lunar space environment and outline the measurements required to address them. These measurements are considered within the framework of the European scientific payload package concept, AstroLEAP (Lunar Environment Analysis Package), which is under study by ESA and the science community.

How to cite: Futaana, Y., Dandouras, I., Fröhlich, P., Genzer, M., Grison, B., Kestilä, A., Pontoni, A., Ranvier, S., Loewe, J. L., Nyman, L., Vorburger, A., Daniel, L. N., Hager, P., McDonald, F., and Cipriani, F. and the AstroLEAP Facility Definition Team and AstroLEAP Study Team: Interdisciplinary exploration science enabled by lunar landers: AstroLEAP sciences, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19727, https://doi.org/10.5194/egusphere-egu26-19727, 2026.

EGU26-19748 | Posters on site | PS1.4

First seismic in-situ characterization of regolith simulants in LUNA 

Brigitte Knapmeyer-Endrun

DLR and ESA are jointly operating the Moon analogue facility LUNA in Cologne, Germany, to provide a venue for end-to-end testing of instruments, experiments, procedures and operations in a controlled, standardized environment. The facility consists of a large-scale testbed filled with mare regolith simulant EAC-1A, nominally to a depth of 60 cm, but extending to 3 m in the so-called deep-floor area (DFA), as well as a smaller dust lab filled to about 60 cm depth with the Lumina250 highland simulant. Both simulants have been characterized with a focus on mineralogical and geological properties, but for EAC-1A, lab data on shear-wave velocities as well as electric properties are also available. For both of these properties, compaction, which is in-situ unknown, plays an important role.

Here, we report on the first attempts of in-situ characterization of the elastic properties of EAC-1A in LUNA by 12 single-station ambient vibration measurements that were analysed in terms of the H/V spectral ratios. In addition to a peak at 0.76 Hz consistently observed at all locations that is related to local geology (sediment-bedrock interface at about 150 m depth), measurements in areas covered by the regolith simulants show additional high-frequency peaks between 12 and 55 Hz, dependent on regolith thickness. As the regolith thickness at each measurement location is known, the common trade-off between layer velocity and thickness in the inversion of the H/V peak frequency is resolved and measurements at different regolith thicknesses can be used to constrain the vertical velocity profile of EAC-1A. However, the task is complicated by strong surface topography as well as the structure of the DFA and buried exploration targets within, which could potentially result in 2D and 3D site effects for some measurement locations. Hence, careful data selection based on the directivity of the observed H/V peaks is performed. First results indicate very similar velocities for both mare and highland simulants, pointing to the dominant effect of granular texture as compared to chemical composition.

We compare fits to the data for different types of velocity laws and also discuss our results in light of the laboratory measurements as well as in comparison to in-situ data from the Moon.

How to cite: Knapmeyer-Endrun, B.: First seismic in-situ characterization of regolith simulants in LUNA, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19748, https://doi.org/10.5194/egusphere-egu26-19748, 2026.

EGU26-20616 | ECS | Orals | PS1.4

An Experimental 2D–3D Dynamic Image Analysis Framework for Particle Shape Characterization and Morphological Analysis of Lunar Regolith Simulants in Multi-Dimensional Morphospaces 

Benedikt Müller, Mohammadhossein Shahsavari, Jonathan Kollmer, Ourania Kounadi, and Matthias Sperl

As human lunar exploration advances through NASA’s Artemis mission and ambitions for a permanent lunar presence grow, understanding lunar regolith is increasingly important. Particle shape plays a pivotal role in governing the behaviour of granular materials, affecting regolith strength, angle of repose, packing density, and interactions with landing spacecraft. Quantitative characterization of lunar regolith particles is therefore essential for mission planning and for the development and validation of adequate simulants used in engineering studies and equipment testing.             

Previous studies have therefore investigated various shape properties of lunar regolith samples and their corresponding simulants using both 2D and 3D techniques. While 2D approaches such as  dynamic (DIA) and static image analysis (SIA) are simple and effective, they do not capture the full 3D geometry of particles and are sensitive to viewing orientation. In contrast, 3D approaches such as laser scanning or X-ray microcomputed tomography (µCT) provide high geometric accuracy but are time-intensive, laborious, and computationally demanding, resulting in a limited number of studies performing 3D shape characterization of lunar regolith simulants. More recently, 3D dynamic image analysis (3D-DIA) has emerged as an intermediate approach, approximating 3D particle geometry from multiple projections. However, only a few setups currently exist, and most rely on proprietary software, limiting transparency, reproducibility, and accessibility.             
Furthermore, extracted shape properties are often analysed individually, overlooking the inherently multi-dimensional nature of particle morphology. Emerging quantitative frameworks, such as morphospaces, are therefore needed to comprehensively capture particle shape and enable systematic, holistic comparison across simulants.

To address the challenge of transparent and reproducible 3D shape characterization of granular particles, we present a novel, low-cost 3D-DIA setup paired with an open-source processing pipeline, which incorporates deep learning–based particle detection and a custom tracking algorithm. The accuracy of derived 3D particle shape descriptors is evaluated against high-resolution µCT scans. Building on the recent introduction of bivariate morphospaces for comprehensive particle shape characterization, we extend this framework by including intermediate-scale particle roundness, thereby establishing a trivariate morphospace that captures all shape properties of powder materials obtainable from imaging data. Distributional patterns within these morphospaces are captured using multi-dimensional Gaussian kernel density estimation (KDE), facilitating quantitative comparison between particle populations via density difference mapping. To further support quantitative assessment across simulants, we introduce the morphological richness (MRic) metric, which condenses the overall morphological diversity of a given simulant into a single scalar value.

To evaluate the proposed framework, 3D particle shape descriptors derived from the 3D-DIA setup were compared with reference µCT measurements. The results show strong agreement and substantial improvement over approximations obtained from single-projection approaches using 2D-DIA and 2D-SIA. Multi-dimensional KDE-based morphospace analysis of EAC-1A, JSC-2A, and NUW-LHT-5M reveals distinct differences in particle shape distributions, further quantified by the MRic metric. These findings demonstrate that the proposed approach provides a robust, reproducible, and scalable method for comprehensive characterization of lunar regolith simulant morphology, supporting the design of more representative simulants and enabling improved understanding of material behaviour in future lunar missions and surface operations.

How to cite: Müller, B., Shahsavari, M., Kollmer, J., Kounadi, O., and Sperl, M.: An Experimental 2D–3D Dynamic Image Analysis Framework for Particle Shape Characterization and Morphological Analysis of Lunar Regolith Simulants in Multi-Dimensional Morphospaces, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20616, https://doi.org/10.5194/egusphere-egu26-20616, 2026.

EGU26-20636 | Orals | PS1.4

Plant-based life support systems: priming plants’ adaptation to the Moon through ionizing radiation within the PRIMO project  

Veronica De Micco, Chiara Amitrano, Sara De Francesco, Antonio Pannico, Marco Durante, Mariagabriella Pugliese, Carmen Arena, Rosanna Caputo, Stefania De Pascale, Serena Perilli, and Marta Del Bianco

Human space exploration is progressively moving toward long-duration missions and permanent human presence on the Moon and Mars. Achieving these ambitious goals requires overcoming major scientific and technological challenges. Among these, habitability requires the development of Bioregenerative Life Support Systems (BLSS), capable of regenerating essential resources and reducing resupply from Earth. Within BLSS, higher plants play a central role, contributing to oxygen production, carbon dioxide removal, water purification, waste recycling, and fresh food supply. The cultivation of plants in space also supports human well-being by alleviating psychological and physiological stress of prolonged isolation and confinement. In fact, the green environments, apart from filtering airborne contaminants, improve psychological relief, emotional stability, and enhance cognitive functions while reducing pain perception. Moreover, the introduction of fresh food in astronauts’ diet contributes to a more balanced diet rich in active compounds, including vitamins, antioxidants, and polyphenols, with both physiological and psychological benefits.

Therefore, plant cultivation in space is increasingly recognized as a key element for crew support by the International Space Exploration Coordination Group (ISECG) within the priority areas, “Life Support and Habitability” and “Crew Health and Performance”.

One of the most critical constraints in extraterrestrial environments is exposure to high levels of ionizing radiation (IR) that significantly influences organism growth and development through molecular alterations, disrupted morphogenesis, and physiological stress responses

Although it is well documented that plants are much more resistant to IR compared to animals, IR can still compromise the efficiency of plants as resource regenerators in BLSS and alter the balance of inputs and outputs among the sub-compartments. Therefore, a thorough understanding of plant responses to radiation is essential for the design and optimization of space greenhouses. However, the exposure to IR at specific doses can enhance plant defense mechanisms, inducing a pre-acclimation response that increases tolerance to subsequent stresses. The PRIMO Project (Priming Radiation-Induced plants’ adaptation to MOon: make an enemy your friend), selected by the European Space Agency (ESA) within the ESA SciSpacE AO - Reserve Pool Of Science Activities for the Moon aims to investigate whether the pre-irradiation of seeds on Earth can enhance plant resistance to the Moon’s environment. The Italian Space Agency (ASI) has funded the preparation of the pre-flight phase of the project, in which seeds of different plant species will be pre-irradiated on Earth using different types and doses of ionizing radiation. Both treated and non-treated (control) seeds will be exposed to the Lunar radiation conditions and reduced gravity throughout the mission duration. After sample recovery, cultivation trials will be conducted under controlled conditions on Earth. Plant performance will be evaluated through growth analysis, transcriptomic profiling, physiological and anatomical assessments, and nutritional quality measurements, providing insights into the feasibility of radiation-based strategies to support sustainable plant cultivation in future lunar BLSS. The approach of PRIMO will allow exploiting the beneficial effects of low-dose radiation to enhance plant tolerance to abiotic stresses, transforming IR from a limiting factor into a potential tool to improve plant resilience to space-related stressors.

How to cite: De Micco, V., Amitrano, C., De Francesco, S., Pannico, A., Durante, M., Pugliese, M., Arena, C., Caputo, R., De Pascale, S., Perilli, S., and Del Bianco, M.: Plant-based life support systems: priming plants’ adaptation to the Moon through ionizing radiation within the PRIMO project , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20636, https://doi.org/10.5194/egusphere-egu26-20636, 2026.

EGU26-22192 | Posters on site | PS1.4

Nanoscale Mid-IR to UV of Lunar Regolith Constituents Through Vibrational Electron Energy Loss Spectroscopy (vibEELS) 

Kenneth Livi, Quentin Ramasse, Demi Kepaptsoglou, Tarunika Ramprasad, Joshua Cahill, Molly McCanta, and Darby Dyar

The anorthite-dominated highlands and the basalt-dominated mare have been bombarded by solar radiation, cosmic rays, charged particles, comets, meteorites, and micrometeorites for over 4.5 billion years, resulting in space weathering at many scales and the collection of interplanetary matter. A majority of the finest fraction (<75 microns) of lunar regolith are endogenous materials: micro- to nano-sized crystalline fragments of the original materials, minerals shocked and amorphized by solar and cosmic radiation, vapor-deposited glass, impact splash, volcanic glass spheres. The exogenous materials include: micro- and nano-scale meteorites and extraterrestrial particles. Despite this conventional microscopy-derived knowledge of the nanoscale, the components of finest fractions of lunar regolith have always been challenging to study with IR and UV spectroscopy due to small grain size, and thermal and space weathering effects that often confound bulk spectra. In fact, until recently, spectroscopy on the individual components at scales of causality (nanometer level) was intractable.

 

We have applied vibrational electron energy-loss spectroscopy to six Apollo samples (three from highlands, three from mare) from four missions, each with differing space weathering maturities (Is/FeO). For highland samples: Apollo 62231 is mature (Is/FeO=91), 61141 sub-mature (56), 61221 immature (8.2). All mare samples are mature: 14259 (85), 15041 (95), and 79221 (80). Identified components in the regoliths include crystalline anorthite, amorphous CaAl2Si2O8(maskelynite) rims with/without iron nanoparticles (FeNPs), olivine, pyroxene, ilmenite, micrometeorites, and glass spheres. This method is employed by a special dedicated scanning transmission electron microscope that generates a monochromated ultrahigh energy resolution electron beam allowing Mid/near IR (MNIR) ‘aloof’ spectral analysis, akin to IR, albeit with a slightly poorer energy resolution, but a much higher spatial localization thanks to the sub-nm electron probe used here. Crystalline anorthite spectra reproduce positions of the five clusters of MNIR absorption peaks (217, 363, 548, 750, 976-1049 cm-1) at slightly lower resolution than FTIR. Loss of crystalline structure causes a split peak at ~1100 cm-1 to broaden, merge, and decrease in intensity. Also, the peak at ~550 cm-1 drops dramatically in intensity in more highly weathered samples. The addition of FeNPs within the amorphous material flattens, or attenuates, the spectra, leaving only the 1100 cm-1 peak. The MIR Christiansen Feature position appears to be affected by crystallinity, glass composition, and abundance of FeNPs at this scale. In the Visible and UV range, "impact" vibEELS collects spectra that document the color absorption changes associated with space weathering as the amount of FeNPs and vitrification increases. The shift towards a reddened slope observed in remote near-IR and UV of bulk samples, is also observed in individual particles that have more FeNPs. The vibEELS data also allows for the determination of the band gap, and therefore, the estimation of the dielectric constant of the weathered surface of regolith particles, which can be used to calculate lunar regolith properties relevant to interpretation of radar wavelengths. 

VibEELS is exquisitely well suited for examination of lunar finest fraction and brings planetary events and materials mixed into this fraction into new focus and perspective. 

How to cite: Livi, K., Ramasse, Q., Kepaptsoglou, D., Ramprasad, T., Cahill, J., McCanta, M., and Dyar, D.: Nanoscale Mid-IR to UV of Lunar Regolith Constituents Through Vibrational Electron Energy Loss Spectroscopy (vibEELS), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22192, https://doi.org/10.5194/egusphere-egu26-22192, 2026.

EGU26-22462 | Posters on site | PS1.4

Mineralogical diversity and soil maturity in the MAJIS/JUICE lunar spectral data  

Maria Cristina De Sanctis, Francesca Altieri, Francesca Zambon, Giuseppe Massa, Stéphane Le Mouélic, Giuseppe Piccioni, François Poulet, Yves Langevin, Clément Royer, Federico Tosi, Ozgur Karatekin, and Alessandro Mura

MAJIS is the Moons and Jupiter Imaging Spectrometer onboard ESA’s Jupiter Icy Moons Explorer (JUICE) mission. It covers the spectral range from 0.5 to 5.56 µm through two spectral channels: the VIS-NIR channel (0.495–2.35 µm) and the IR channel (2.28–5.56 µm), with up to 640 spectral samples per channel. The main scientific goals of MAJIS are to investigate the surface composition and physical properties of the Jovian icy satellites by detecting ices, salts, organics, and rocky materials [1].

The JUICE mission was launched in April 2023 and will arrive at Jupiter in July 2031. During the cruise phase, JUICE performed observations of the Moon and Earth thanks to a double flyby (Lunar-Earth Gravitational Assist, LEGA) in August 2024, reaching a minimum altitude of 750 km for the Moon and 6100 km for Earth. This provided a unique opportunity to validate MAJIS’s technical and scientific performance after launch [2, 3].

On the Moon, MAJIS observed equatorial regions in Mare Tranquillitatis, Mare Fecunditatis, and neighbouring highland terrains, confirming its capability to detect and map lunar mineralogical diversity and soil maturity [2, 4]. Here, we focus on regions including Duke Island and the Ruin Basin in Mare Tranquillitatis, and the Messier Crater rays in Mare Fecunditatis. Detections of glass, pyroxene and olivine in other locations are also discussed.

 

This work has been developed under the ASI-INAF agreement n. 2023-6-HH.0.

 

[1] Poulet et al., 2024, SSR. [2] Poulet et al., 2026, Ann. Geo., submitted. [3] Langevin et al., 2026, Ann. Geo., submitted. [4] Zambon et al., 2026, Ann. Geo., submitted.

How to cite: De Sanctis, M. C., Altieri, F., Zambon, F., Massa, G., Le Mouélic, S., Piccioni, G., Poulet, F., Langevin, Y., Royer, C., Tosi, F., Karatekin, O., and Mura, A.: Mineralogical diversity and soil maturity in the MAJIS/JUICE lunar spectral data , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22462, https://doi.org/10.5194/egusphere-egu26-22462, 2026.

EGU26-22820 | Orals | PS1.4

Overview of the NASA instruments onboard Blue Ghost Mission 1 

Maria Banks and the EDS team, LEXI team, LISTER team, LMS team, LPV team, LuGRE team, NGLR team, RadPC team, RAC team, SCALPSS team

Blue Ghost Mission 1 (BGM1), or NASA CLPS (Commercial Lunar Payload Services) Task Order (TO) 19D, delivered ten NASA science and technology instruments to the lunar surface (18.5623°N, 61.8103°E) in 2025. All NASA payloads successfully activated and performed operations on the Moon:

LuGRE (Lunar GNSS Receiver Experiment) acquired and tracked Global Navigation Satellite System (GNSS) signals from GPS and Galileo constellations and calculated instantaneous navigation “fixes” enroute to and on the Moon’s surface for the first time. LuGRE demonstrated that GNSS signals can be used to support navigation in cislunar space and at the Moon.

RadPC (Radiation Tolerant Computer System) successfully operated through Earth’s Van Allen belts, in transit to and in lunar orbit, and on the lunar surface. RadPC verified solutions to mitigate radiation effects on computers that could make future missions safer for equipment and more cost effective.

EDS (Electrodynamic Dust Shield) successfully lifted and removed lunar regolith from surfaces using electrodynamic forces demonstrating a promising solution for dust mitigation on future lunar and interplanetary surface operations.

SCALPSS (Stereo Cameras for Lunar Plume-Surface Studies) captured more than 9,000 images including during the spacecraft’s descent to the surface, providing insights into the effects engine plumes have on the surface. The payload also operated on the surface during the lunar day, during the lunar sunset, and into the lunar night.

LISTER (Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity) is now the deepest robotic planetary subsurface thermal probe, drilling and acquiring thermal measurements at eight depths down to ~1-m depth. LISTER provided a first-time demonstration of robotic thermal measurements at varying depths.

LMS (Lunar Magnetotelluric Sounder) determined that the subsurface electrical conductivity profile beneath the Blue Ghost lunar lander is very similar to that below the Apollo 12 site. This implies that the widespread basaltic volcanism of the western nearside was not powered by regional enhancement of heat-producing elements, but was likely a consequence of easier eruption through thinner crust.

LEXI (Lunar Environment heliospheric X-ray Imager) captured X-ray images to study the interaction of the solar wind and Earth’s magnetic field to provide insights into how space weather and other cosmic forces surrounding Earth affect the planet. LEXI also observed density profiles of the lunar exosphere through solar wind charge-exchange emission.

NGLR (Next Generation Lunar Retroreflector) has successfully reflected and returned laser light for thousands of individual range measurements from multiple Lunar Laser Ranging Observatories (LLROs) on Earth. Measurements utilizing NGLR will enable precise measurements of the Moon’s shape and distance from Earth, expanding our understanding of the Moon’s inner structure. 

LPV (Lunar PlanetVac) was deployed on the lander’s surface access arm and collected, transferred, and sorted lunar regolith particles using pressurized nitrogen gas, including acquiring regolith without physically touching the lunar surface. LPV successfully demonstrated a low-cost, low-mass solution for future robotic sample collection.

RAC (Regolith Adherence Characterization) examined how regolith sticks to a range of materials exposed to the lunar environment. Results can help test, improve, and protect spacecraft, spacesuits, and habitats from abrasive lunar dust.

How to cite: Banks, M. and the EDS team, LEXI team, LISTER team, LMS team, LPV team, LuGRE team, NGLR team, RadPC team, RAC team, SCALPSS team: Overview of the NASA instruments onboard Blue Ghost Mission 1, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22820, https://doi.org/10.5194/egusphere-egu26-22820, 2026.

Stable isotopes of oxygen and hydrogen are a powerful multipurpose tool widely used across multiple disciplines in Earth and Planetary sciences. In hydrology, δ18O and δ2H in the water molecule are commonly used in stream water source apportionment and transit time analyses. In paleoclimate research, ice core water isotope records are used as a temperature proxy, documenting past climate variability over hundreds of thousands of years. Oxygen and hydrogen isotopes are also versatile fingerprints for retracing the formation of planets and other celestial bodies.

These examples should not obscure the fact that many unknowns and uncertainties remain inherent to the use of stable isotopes of O and H as tracers and fingerprints of processes in terrestrial and extra-terrestrial environments. To this date, only a few experimental studies have investigated water ice sublimation rates and the effect of isotopic fractionation processes – notably on water ice under lunar environmental conditions.

Here we present results from a combined experimental and modelling approach. With an instrumental set-up developed at LIST, we simulate the sublimation of water ice under extreme environmental conditions (very high vacuum and/or very low temperatures) with the goal of exploring O-H isotopic fractionation processes in both (extreme) terrestrial and extraterrestrial environments. An understanding of these processes is necessary for interpreting the isotope signatures of water in planetary exploration missions, such as ESA’s PROSPECT project for lunar exploration, and in terrestrial hydrology of cold regions.

The current experimental setup consists of a sublimation chamber capable of operating at pressures down to 10⁻⁶ Pa and temperatures as low as 110 K, with high stability and control over sublimation conditions. The system can simulate controlled environments for the phase transition of water (ice-vapor), isotopic fractionation, and the movement of water vapor across different phases of the experimental run. This includes transferring gas to a series of parallel cold traps, analyzing isotopic content using laser spectroscopy.

We have developed a stochastic lagrangian numerical model to verify the existing theories of phase transition, diffusion, and O-H isotopic fractionation based on the Langevin equation. The model allows for sublimation, diffusive transport, and condensation of water and its isotopes through an isothermal domain representing the volume of the experimental prototype. Lagrangian models are highly adaptive for handling complex boundary conditions and well-suited for solving fluid mechanics problems with various types of particles.

A sensitivity analysis of the model using different sublimation temperatures shows consistent results with our experimental data. Results obtained from the dual isotope analysis (δ¹⁸O and δ²H) of ice samples obtained from Greenland Summit Precipitation (GRESP) and Antarctica snow show trends consistent with theoretical predictions and meteoric water line, suggesting that the setup is operating reliably. Observed deviations in the isotopic compositions indicate influences from environmental variables such as humidity, pointing towards the need for tighter control and validation. Our experimental set-up lays a foundation for further investigations into the problems of fast diffusion, non-equilibrium thermodynamics, and the isotopic signature of water.

How to cite: Kumawat, M., Barnich, F., Pfister, L., Zehe, E., and Hadler, K.: Water ice sublimation and O-H isotopic fractionation in terrestrial and extraterrestrial environments: new insights gained from numerical modelling and laboratory experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23186, https://doi.org/10.5194/egusphere-egu26-23186, 2026.

EGU26-3821 | Orals | ESSI2.7

Reproducible and Scalable cloud-native EO data analysis using openEO  

Pratichhya Sharma, Hans Vanrompay, and Jeroen Dries

Earth Observation (EO) data plays a crucial role in research and applications related to environmental monitoring, enabling informed decision-making. However, the continuously increasing volume and diversity of EO data, distributed across multiple platforms and varying formats, pose challenges for easy access and the development of scalable and reproducible workflows.

openEO addresses these challenges by providing a community-driven, open standard for unified access to EO data and cloud-native processing capabilities. It supports researchers to develop interoperable, scalable and reproducible workflows that can be executed using various programming languages (Python, R or JavaScript).

openEO has become a cornerstone technology across major initiatives in agriculture, natural capital accounting, and land-cover monitoring. In ESA’s WorldCereal project, it provides the scalable framework needed to process global Sentinel-1 and Sentinel-2 time series and integrate advanced machine-learning models, enabling dynamic 10-meter cropland and crop-type maps. It also supports the Copernicus Global Land Cover service and its tropical forestry component by delivering consistent and repeatable processing chains for annual 10-meter land-cover products, which are crucial for policy reporting and SDG monitoring. Beyond land cover, openEO supports efforts like ESA's World Ecosystem Extent Dynamics project by creating reproducible ecosystem-extent mapping and change detection maps — key elements for biodiversity and environmental management.

Building on this foundation, the openEO Federation, now integrated within the Copernicus Data Space Ecosystem (CDSE), provides seamless access to distributed Earth observation data and processing resources through a single, unified interface. By connecting multiple backends, it removes the need to juggle separate accounts or APIs and enables cross-platform workflows over datasets hosted by platforms such as Terrascope and CDSE.

openEO also strongly supports FAIR (Findable, Accessible, Interoperable, Reusable) principles. It exposes rich metadata, relies on standardised processes, and encourages the use of reusable workflow definitions. This promotes transparency, reproducibility, and the sharing of algorithms and data across research and operational communities. The approach has been validated in several large-scale implementations, including ESA’s WorldCereal and the JRC’s Copernicus Global Land Cover and Tropical Forestry Mapping and Monitoring Service (LCFM), demonstrating its maturity for both research and production environments.

By enabling reusable, federated, and reproducible Earth observation workflows, openEO is helping to build a more interoperable and efficient computational ecosystem, one that supports scalable innovation, collaboration, and long-term operational monitoring. Therefore, in this session, we aim to spark discussion on how openEO enables federated, FAIR-compliant, and reproducible workflow approaches for large-scale Earth observation applications.

How to cite: Sharma, P., Vanrompay, H., and Dries, J.: Reproducible and Scalable cloud-native EO data analysis using openEO , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3821, https://doi.org/10.5194/egusphere-egu26-3821, 2026.

EGU26-5728 | ECS | Posters on site | ESSI2.7

Parallel HPC workflow orchestration with Nextflow, supported by CI/CD and containerization tools for global high resolution evaporation modelling 

Joppe Massant, Oscar Baez-Villanueva, Kwint Delbaere, Diego Fernandez Prieto, and Diego Miralles

The Global Land Evaporation Amsterdam Model (GLEAM) estimates daily land evaporation using a wide range Earth observation forcing datasets. In the project GLEAM-HR funded by the European Space Agency (ESA), we aim to create a global high-resolution daily evaporation dataset at 1 km for a period of eight years (2016–2023). To produce high-resolution evaporation estimates, all forcing data must be processed at 1 km resolution, requiring substantial computational resources. As the complete high-resolution forcing data no longer fits within the memory capacity of single HPC nodes, parallelization tools are necessary. To achieve this parallelization in a seamless way, a workflow orchestration ecosystem is designed that leverages the use of Zarr, Apptainer and Nextflow.

The Zarr ecosystem allows for easily writing to a dataset in parallel. Nextflow is an orchestration tool that allows dynamic job submissions, where the configuration of jobs can depend on the outcome of earlier jobs, such as the spatial domain to be processed. Apptainer is a containerization tool developed for HPC environments, allowing a “build once, deploy anywhere” approach. Combining these tools allows building a workflow orchestration environment that enables the automation of these parallel workflows while optimizing the job sizes for a given HPC environment.

The use of containers allows this workflow to be ported to different hardware without the need to set up all the environments again, making the designed workflow fully reproducible independent of the computing environment. Combining this with Continuous Integration and Continuous Delivery (CI/CD) practices to automate the container building and deployment, code development and workflow execution can be cleanly separated.

In a first test case, this processing workflow is used to produce global datasets of LAI, FPAR and vegetation cover fractions at 1 km resolution.  Future work focuses on the extension of this workflow to the other forcing datasets and the entire pipeline execution.

How to cite: Massant, J., Baez-Villanueva, O., Delbaere, K., Fernandez Prieto, D., and Miralles, D.: Parallel HPC workflow orchestration with Nextflow, supported by CI/CD and containerization tools for global high resolution evaporation modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5728, https://doi.org/10.5194/egusphere-egu26-5728, 2026.

EGU26-6238 | ECS | Posters on site | ESSI2.7

A prototype Open-Source data-processing pipeline to efficiently combine in-situ data with remote-sensing observations of the Earth 

Robert Reinecke, Annemarie Bäthge, David Noack, Matthias Zink, Simon Mischel, and Stephan Dietrich

In situ and remote sensing data are crucial in earth sciences, as they provide complementary perspectives on environmental phenomena. In situ data, collected directly from the Earth’s surface, offer high accuracy and detailed insights into local conditions, enabling precise measurements of variables such as soil moisture, temperature, and pollutant levels. Conversely, remote sensing data provides for extensive spatial coverage and the ability to monitor changes over time across vast areas, capturing large-scale patterns and trends that in situ data alone cannot reveal. By combining these two data sources and automatically preprocessing them into Analysis-Ready Data, researchers can enhance scientific insights, improve the robustness of machine learning applications, and refine models used to predict environmental changes or assess the impacts of human activity on natural systems. This integrated approach promotes a more comprehensive understanding of complex Earth processes, enabling better-informed decision-making and effective management strategies for sustainable development. However, preprocessing and combining in situ data from different sources can be highly complex, especially for global datasets. Joining this data with remotely sensed products may require substantial computational resources, given the increased number of observational records and high temporal resolutions. Here, we present a prototype of such a pipeline, CULTIVATE, an open-source data-processing pipeline that efficiently cleans in situ records and combines them with remote sensing data to create an automatically curated database. As new in situ data records are inserted, CULTIVATE updates only those records in the final database. In this presentation, we showcase CULTIVATE for over 200,000 global groundwater well observation time series that are merged with an extensive list of other time-series products, and we show how data curators can interact with the data processing pipeline. We further discuss how this prototype can serve as a blueprint for future architecture development for Research Data Infrastructures, how we can implement and enforce international standards, and how we can enable global datacenters to utilize automated data preparation in operational settings.

How to cite: Reinecke, R., Bäthge, A., Noack, D., Zink, M., Mischel, S., and Dietrich, S.: A prototype Open-Source data-processing pipeline to efficiently combine in-situ data with remote-sensing observations of the Earth, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6238, https://doi.org/10.5194/egusphere-egu26-6238, 2026.

EGU26-7115 | ECS | Posters on site | ESSI2.7

STeMP: Spatio-Temporal Modelling Protocol 

Jan Linnenbrink, Jakub Nowosad, Marvin Ludwig, and Hanna Meyer

Spatio-temporal predictive modelling is a key method in the geosciences. Often, machine-learning, which can be applied to complex, non-linear and interacting relationships, is preferred over classical (geo)statistical models. However, machine-learning models are often perceived as "black boxes", meaning that it is hard to understand their inner workings. Furthermore, there are several pitfalls associated with the application of machine-learning models in general, and spatio-temporal machine-learning models in particular. This might, e.g., concern the spatial autocorrelation inherent in spatial data, which complicates data splitting for model validation. 

Following from this, it is key to transparently report spatio-temporal models. Transparent reporting can facilitate interpreting, evaluating and reproducing spatio-temporal models, and can be used to determine their suitability for a specific research question. Standardized model protocols are particularly valuable in this context, as they document model parameters, decisions and assumptions. While such protocols exist for machine-learning models in general (e.g., Model Cards, REFORMs), as well as for specific domains like species distribution modelling (ODMAP), such protocols are lacking in the general field of spatio-temporal modelling. 

Here, we present ideas for STeMP (Spatio-Temporal Modelling Protocol), a protocol for spatio-temporal models that fills this gap. The protocol is designed to be beneficial for all parties involved in the modeling process, including model developers, maintainers, reviewers, and end-users. The protocol is implemented as a web application and is structured in three sections: Overview, Model and Prediction. The Overview section contains general metadata, while the following two sections go into more detail. The Model section includes modules describing, for example, the predictors, model validation procedures, and software. The optional Prediction section contains information about the prediction domain, map evaluation, and uncertainty assessment.

To make the protocol useful during model development, warnings are raised when common pitfalls are encountered (e.g., if an unsuitable cross-validation strategy is used). These warnings can be automatically retrieved from a filled protocol, spotlighting potential issues and helping authors and reviewers. Moreover, we provide the optional possibility to generate automated reports and also inspection figures from user-provided inputs (e.g., from model objects as well as from training and test data sets). The protocol is hosted on GitHub (https://github.com/LOEK-RS/STeMP) and hence open to flexible incorporation of feedback from the broader community.

With our presentation, we aim to encourage the discussion of our proposed model report in the spatio-temporal modelling community.

How to cite: Linnenbrink, J., Nowosad, J., Ludwig, M., and Meyer, H.: STeMP: Spatio-Temporal Modelling Protocol, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7115, https://doi.org/10.5194/egusphere-egu26-7115, 2026.

EGU26-9928 | Orals | ESSI2.7

Research data infrastructure evolution for handling km scale simulations of a warming world 

Kameswarrao Modali, Karsten Peters-von Gehlen, Fabian Wachsmann, Florian Ziemen, Carsten Hinz, Rajveer Saini, and Siddhant Tibrewal

With the advancement of technical capabilities, Earth System Models (ESM) are rapidly moving toward much higher spatial resolutions - down to kilometer scale - to better capture key processes and feedbacks needed for robust climate impact assessments. This growing model complexity places significant demands on data infrastructures, which must evolve to support widespread application of  high-resolution simulations.

This evolution is needed across various stages of the ESM simulation data life cycle, right from the choice of the variables that need to be part of the simulation output, the format of the output, residence period and transfer of the data across various active storage tiers and the final movement to the cold storage tier (tapes) for long time archival. Also tools to handle the discoverability of these data must be developed and implemented. The evolution of the infrastructure also must take hardware constraints into account and should ideally be in line with the FAIR principles.

As part of the Warm World Easier project, these developments were the adaptation of the model output to zarr, a cloud native format, the development of bespoke tools like ‘zarranalyzer’ to handle the movement of the data across storage tiers by creating tarballs suitable also for the tapes, creating reference files for these tarballs in parquet format to summarize the entire dataset and the inception of these into a metadata catalog following the SpatioTemporal Asset Catalog (STAC) standard. Finally, a virtual machine to host the STAC catalog with appropriate access rights for the data providers and data curators within the federated structure, as well as the end users, was set up. 

Applying this data handling concept to km-scale ESM data bridges the gap between infrastructures that produce flagship datasets and those that enable their efficient and reliable reuse by the community. For example, data generated at large, compute-focused HPC centers with limited storage could be transferred to partner centers that provide specialized data services for long-term access and reuse. 

Through the federated and seamless setup of the research data infrastructure, data handling matters are abstracted away from the data users. Hence, the developed setup provides an end to end solution, achieving the objective of providing the km scale ESM simulation output to a broader scientific community tackling the urgent societal problems arising due to a warming planet.

How to cite: Modali, K., Peters-von Gehlen, K., Wachsmann, F., Ziemen, F., Hinz, C., Saini, R., and Tibrewal, S.: Research data infrastructure evolution for handling km scale simulations of a warming world, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9928, https://doi.org/10.5194/egusphere-egu26-9928, 2026.

EGU26-11128 | Orals | ESSI2.7

Antflow: Simplifying Workflow Sharing and Execution for Digital Twins 

Nicolas Choplain and Gaudissart Vincent

Antflow is a next-generation orchestration and publication framework designed to streamline the operational deployment of Earth Observation (EO) processing workflows, particularly within Digital Twin environments. By automating the transformation of scientific code into interoperable, shareable, and scalable services, Antflow removes the traditional barriers between algorithm development and production-grade execution.

At its core, Antflow enables scientists and developers to publish complex workflows directly from their Git repositories, using OGC Earth Observation Application Packages (EOAP) as the workflow definition mechanism. These EOAP descriptions allow Antflow to instantly expose workflows as OGC API Processes services, enriched with dynamic user interfaces and STAC-compliant cataloguing of outputs. This ensures that every workflow - no matter how experimental or mature - can be discovered, reused, and integrated across Digital Twin platforms.

Antflow’s hybrid orchestration engine distributes tasks across heterogeneous computing environments, from HPC clusters to cloud-native nodes. Git-based lineage guarantees traceability and scientific integrity, while integrated multi-provider retrieval mechanisms (EODAG) simplify access to EO data sources.

A key strength of Antflow is its ability to generate interactive user interfaces automatically. These interfaces allow domain experts, integrators, and end-users to parameterize, run, and monitor workflows through clean, intuitive views.

Antflow is currently used across several projects (CNES Digital Twin Factory, OGC Open Science Persistent Demonstrator). It acts as a middleware layer that bridges algorithm design, operational integration, and stakeholder consumption. By standardizing workflow publication, ensuring reproducibility, and supporting scalable execution, it accelerates the deployment of modelling chains such as 3D environmental reconstruction, forecasting, and multi-sensor analysis workflows.

How to cite: Choplain, N. and Vincent, G.: Antflow: Simplifying Workflow Sharing and Execution for Digital Twins, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11128, https://doi.org/10.5194/egusphere-egu26-11128, 2026.

EGU26-11759 | ECS | Posters on site | ESSI2.7

Accelerating Earth System Workflows with In Situ Workflow Task Management 

Manuel Giménez de Castro Marciani, Mario Acosta, Gladys Utrera, Miguel Castrillo, and Mohamed Wahib

Modern experimentation with Earth System Models (ESMs) is accelerated by the employment of automated workflows to handle the multiple steps such as simulation execution, post-processing, and cleaning, all while being portable and tracking provenance. And when executing on shared HPC platforms, users usually face long queue times, which increase the time to solution. The community has proposed to aggregate workflow tasks into a single submission in order to save in queue time with promising results. But by doing this the workflow manager has to deal with the remote task execution that otherwise would have been done by the HPC scheduler.

Therefore, we propose to integrate two workflow managers to create a versatile and general solution for the execution of these aggregated workflows: one that orchestrates the workflow globally and another that is in charge of running tasks within an allocation, which we refer to as "in situ."

In this work, we performed a qualitative and quantitative comparison of three suitable and representative workflow and workload managers running in situ, HyperQueue, Flux, and PyCOMPSs, on three of the top 20 HPCs: Lumi, MareNostrum 5, and Fugaku. We evaluated the portability and setup, failure tolerance, programmability, and provenance tracking of each of the tools in the qualitative part. In the quantitative part, we measured total runtime, task runtime, CPU and memory usage, disk write, and node imbalance of workflows running a memory-bound, a CPU-bound, and an IO-intensive application.

Our initial results yield recommendations to the community as to which workflow manager to use in situ. HyperQueue's easy installation and portability makes it the best solution for non-x86 platforms. Flux had the easiest running setup due to its preparedness to run nested in Slurm. Finally, PyCOMPSs is the only tool out of the three to provide provenance tracking with RO-Crates.

How to cite: Giménez de Castro Marciani, M., Acosta, M., Utrera, G., Castrillo, M., and Wahib, M.: Accelerating Earth System Workflows with In Situ Workflow Task Management, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11759, https://doi.org/10.5194/egusphere-egu26-11759, 2026.

EGU26-12058 | ECS | Orals | ESSI2.7

Optimizing the Destination Earth Workflow with in situ HPC Task Orchestration 

Pablo Goitia, Manuel Giménez de Castro Marciani, and Miguel Castrillo

Traditionally, climate simulations are executed on High-Performance Computing (HPC) platforms, organized in workflows that involve all the steps for the complete execution of the model, data processing, and management tasks. With the sustained increase in the computing capacity of these machines over the years, the accuracy and resolution of climate simulations have reached levels never seen before.

In this context, the European Commission launched the Destination Earth initiative, aimed at developing a digital twin of the Earth for the adaptation to climate change. This initiative seeks to operationalize the running of very high-resolution climate simulations that are coupled with applications that consume their data as it is produced. In order to address the challenge of processing the hundreds of terabytes that each single simulation involves, the ClimateDT project implemented a data streaming approach. This means that any delay between the production time of the climate model data and the subsequent consumption by the post-processing applications results in a workflow misalignment, leading to unacceptable delays in the total execution time. This poses unprecedented challenges on the workflow management side.

One of the main causes of the misalignments that commonly occur lies in the long time that each of the many thousands of tasks of the workflow spends in the queues of the HPC job schedulers, such as Slurm. To address this issue, the community proposed to aggregate workflow tasks into a single submission to the HPC without altering their execution logic—a technique known as task aggregation. Previous studies have demonstrated the effectiveness of this approach for climate workflows, yielding promising results. However, the current implementation is limited, as the task execution within an allocation still relies on the workflow manager, which is not able to perform the fine-grained workflow orchestration that a dedicated tool could do in a convenient way.

To overcome this limitation, we propose in this work to integrate existing HPC software into the Autosubmit Workflow Manager to enable in situ orchestration of aggregated tasks, such as the renowned Flux Framework and Parsl. This integration aims to abstract both developers and users from the complexity of managing supercomputing resources, providing an easy-to-use interface. The proposed approach is validated using the Destination Earth workflow to enable more complex, structured forms of task aggregation while reducing queue times in large-scale simulations.

How to cite: Goitia, P., Giménez de Castro Marciani, M., and Castrillo, M.: Optimizing the Destination Earth Workflow with in situ HPC Task Orchestration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12058, https://doi.org/10.5194/egusphere-egu26-12058, 2026.

EGU26-14853 | ECS | Posters on site | ESSI2.7

AutoML: A Flexible and Scalable HPC Framework for Efficient Machine Learning in Atmospheric Modelling 

Isidre Mas Magre, Hervé Petetin, Alessio Melli, James Petticrew, Michael Orieux, Miguel Hortelano, Luiggi Tenorio, and David Mathas

The integration of Machine Learning (ML) into Earth System Sciences has revolutionized predictive modeling. However, the transition from local prototyping to large-scale deployment is often hindered by fragmented codebases and the manual overhead of managing complex hyperparameter tuning on High-Performance Computing (HPC) clusters. We present AutoML, a framework developed to automate and standardize the ML lifecycle in HPC environments by leveraging the open-source Autosubmit workflow manager.

AutoML employs a configuration-driven architecture that decouples model logic from workflow execution. By utilizing Autosubmit’s proven capability to handle complex dependencies and remote HPC environments, AutoML allows researchers to scale experiments—from initial prototyping to production-level global pipelines—through a single configuration file. This approach directly addresses the challenge of experiment reproducibility and efficiency within ML projects. The framework automates critical steps in the typical ML workflow, including hyperparameter search space optimization, multi-node distributed training, and dynamic resource allocation on heterogeneous HPC architectures.

We demonstrate the framework’s utility through Atmospheric Composition applications at the Barcelona Supercomputing Center (BSC). By providing a standardized structural template AutoML fosters collaboration and ensures that advancements in machine learning for atmospheric science are scalable, computationally efficient, and transferable across research lines.

How to cite: Mas Magre, I., Petetin, H., Melli, A., Petticrew, J., Orieux, M., Hortelano, M., Tenorio, L., and Mathas, D.: AutoML: A Flexible and Scalable HPC Framework for Efficient Machine Learning in Atmospheric Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14853, https://doi.org/10.5194/egusphere-egu26-14853, 2026.

EGU26-15002 | Orals | ESSI2.7

Toward Federated Agentic Workflows for Numerical Weather Prediction With Chiltepin 

Christopher Harrop and Isidora Jankov

The development of efficient, scalable, and interoperable workflow management systems is critical for supporting reproducible research to drive the scientific advancement of earth system modeling capabilities. Many workflow systems targeted for earth system science have been developed to meet that challenge, each having similar capabilities as well as some unique strengths. However, the earth system modeling community now faces additional challenges that impose new requirements. The landscapes of both high performance computing (HPC) environments and numerical modeling are evolving rapidly. HPC systems are composed of a growing diversity of hardware architectures that may be hosted on-prem or by a variety of cloud vendors. Earth model system components are also increasing in diversity as research to augment or replace traditional physics based models with machine learning models progresses. Additionally, a growing diversity of end-users with varying levels of knowledge and expertise require agentic workflows that can respond to their requests. A consequence of this rapid growth in diversity is a growing need to run workflows that span multiple systems in order to optimize data locality and access to resources that maximize performance of specific model components. The availability of, and requirement for, diversity naturally leads to a requirement for federated workflows that effectively harness the computational power of a diverse set of resources distributed both geographically and across multiple administrative domains. In this presentation, we introduce and report our progress with the development of Chiltepin, the first known federated numerical weather prediction workflow system within the National Oceanic and Atmospheric Administration (NOAA). Chiltepin is designed to address key challenges in numerical modeling, particularly those related to sustainable progress in a changing NWP landscape characterized by increasing diversity of technologies and use of high-performance computing resources distributed across both geographical and administrative boundaries.

How to cite: Harrop, C. and Jankov, I.: Toward Federated Agentic Workflows for Numerical Weather Prediction With Chiltepin, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15002, https://doi.org/10.5194/egusphere-egu26-15002, 2026.

EGU26-17077 | Posters on site | ESSI2.7

ARCA: A Scalable and Reproducible AI-Driven Workflow Platform for Climate Change and Natural Hazard Applications 

Maria Mirto, Marco De Carlo, Shahbaz Alvi, Shadi Danhash, Antonio Aloisio, and Paola Nassisi

Earth System Sciences (ESS) are increasingly characterized by large data volumes and high computational demands, which make complex analyses difficult to manage using ad hoc or manual solutions. This challenge is amplified when heterogeneous data sources, such as Internet of Things (IoT) infrastructures including wireless sensor networks, video cameras and drones, must be combined with high-performance computing (HPC) environments for climate modelling and advanced artificial intelligence (AI) algorithms.

The ARCA (Artificial Intelligence Platform to Prevent Climate Change and Natural Hazards) project, funded by the Interreg IPA ADRION Programme, was designed to respond to these challenges by providing a practical, workflow-based platform aimed at supporting climate change and natural hazard applications and, ultimately, reducing their impacts. The main objective of ARCA is to strengthen the cross-border operational capacity of stakeholders across the Adriatic–Ionian region, involving Italy, Croatia, Montenegro, Albania, Serbia and Greece. The platform supports the monitoring of forest ecosystems through AI-based tools, enabling continuous observation of forest areas and the prediction of multiple natural hazards, including droughts, wildfires and windstorms.

ARCA is built on a modular architecture centered on scientific workflows, which orchestrate multiple-type data ingestion, processing, analysis and AI model execution in a consistent and reproducible manner. The platform integrates big data technologies, workflow management systems and AI components, allowing complex processing chains to be automated while ensuring full traceability of data provenance, computational steps and model configurations. This approach supports FAIR principles and promotes the reuse of data and workflows across different applications and computing environments.

A key strength of ARCA lies in its ability to shield users from much of the underlying technical complexity, such as heterogeneous computing resources, access constraints and large data volumes, while still enabling scalable AI-driven analyses. As a result, researchers and practitioners can focus on scientific and operational questions related to climate impacts and hazard prevention rather than on low-level technical orchestration. In this contribution, we present the overall ARCA architecture together with selected use cases, illustrating how workflow-based approaches can effectively support scalable, transparent and reproducible ESS research in a multinational and federated context like the Adriatic–Ionian region.

How to cite: Mirto, M., De Carlo, M., Alvi, S., Danhash, S., Aloisio, A., and Nassisi, P.: ARCA: A Scalable and Reproducible AI-Driven Workflow Platform for Climate Change and Natural Hazard Applications, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17077, https://doi.org/10.5194/egusphere-egu26-17077, 2026.

EGU26-17974 | Orals | ESSI2.7

Multi-target process dispatch on the European Digital Twin of the Ocean  

stella valentina Paronuzzi ticco, Quentin Gaudel, Alain Arnaud, Jerome Gasperi, Mathis Bertin, and Victor Gaubin

The EDITO platform serves as the foundational framework for building the European Digital Twin of the Ocean. It seamlessly integrates oceanographic data and computational processes (non-interactive remote functions that take input and produce output) on a single platform that relies on both cloud and HPC (EuroHPC) resources. In this context, EDITO already provides many processes, such as OceanBench model evaluation and the ML-based GLONET 10-day forecast. To make scientists' work easier, we have developed a new way of generating processes on EDITO. We will use OceanBench evaluation as an example of a process that can be dispatched by the user on multiple targets, seamlessly handling the technical complexity of dealing with different hardware (cloud CPUs/GPUs, HPC, etc.). In our presentation we will explain how EDITO contributors will benefit from this new method of generating processes.   

How to cite: Paronuzzi ticco, S. V., Gaudel, Q., Arnaud, A., Gasperi, J., Bertin, M., and Gaubin, V.: Multi-target process dispatch on the European Digital Twin of the Ocean , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17974, https://doi.org/10.5194/egusphere-egu26-17974, 2026.

EGU26-18841 | ECS | Posters on site | ESSI2.7

Efficient large-scale data structuring to support Earth System Science analytics workflows 

Donatello Elia, Gabriele Tramonte, Cosimo Palazzo, Valentina Scardigno, and Paola Nassisi

The amount of data produced by Earth System Model (ESM) is continuously growing, driven by their higher resolution and complexity. Approaches for efficient data access, management, and analysis are, thus, needed now more than ever to tackle the challenges related to these large volumes. Moreover, data generated by ESM simulations could be organized in a way that is not the most effective for data analytics, slowing down scientists’ productivity. In this context, novel data formats and proper chunking strategies can significantly speed up access and processing of Earth system data and, in turn, the whole analysis workflow. 

In the scope of ESiWACE3 - Centre of Excellence in Simulation of Weather and Climate in Europe - we experimented the impact of different data formats and chunking configurations on high-performance data analytics operations/workflows. In particular, we evaluated performance of the well-known NetCDF format and the more recent cloud-native Zarr format, which is being increasingly used in Earth Science data analytics workflows and machine learning applications. Results show that the use of a proper data format and structure can noticeably reduce the time required for executing these analytics workflows, provided the structure is carefully tuned (e.g., chunking).

The work presents the main outcomes of such evaluation and how we are exploiting this knowledge to enhance Earth system data management workflows. In particular, the results achieved have contributed to enabling a more efficient access, delivery and analysis of large-scale data in CMCC’s tools and services, which are involved in different initiatives, including the ICSC - National Centre on High Performance Computing, Big Data and Quantum Computing.

How to cite: Elia, D., Tramonte, G., Palazzo, C., Scardigno, V., and Nassisi, P.: Efficient large-scale data structuring to support Earth System Science analytics workflows, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18841, https://doi.org/10.5194/egusphere-egu26-18841, 2026.

EGU26-19451 | ECS | Posters on site | ESSI2.7

Making Kilometer-Scale Earth System Model (ESM) simulations usable: A workflow approach from European Eddy RIch ESMs (EERIE) project. 

Chathurika Wickramage, Fabian Wachsmann, Jürgen Kröger, Rohith Ghosh, and Matthias Aengenheyster

Kilometer-scale global climate simulations are now generating petabytes of output at such a rapid pace that data production is surpassing data standardization. Central ESM infrastructures have traditionally followed a “data warehouse” approach: extensive preprocessing, quality control, and formatting are performed before users receive self-describing, FAIR-aligned files. While this delivers highly standardized and interoperable products, it also creates a growing bottleneck, computationally and organizationally, so that routine actions like checking variables, extracting a region and time slice, or comparing experiments can become slow, and hard to reproduce in practice. The EERIE project (https://eerie-project.eu/about/) is a clear example: its eddy-rich Earth System Models generate detailed and valuable output, but at a scale and pace that overwhelms traditional file-by-file workflows and delays usable access.

At DKRZ, we address this with an end-to-end workflow that transforms raw EERIE model output into analysis-ready datasets (ARD) that are easy to discover, subset, and analyze without requiring users to copy or download terabytes of files. The central element of this workflow is to create virtual Zarr datasets of the raw model output received from the modeling groups, by extracting chunk information and storing them in the kerchunk format with VirtualiZarr (https://virtualizarr.readthedocs.io/en/stable/index.html). These native-grid virtual datasets are published through both an intake catalog (https://github.com/eerie-project/intake_catalogues) and a STAC (SpatioTemporal Asset Catalog; https://discover.dkrz.de/external/stac2.cloud.dkrz.de/fastapi/collections/eerie?.language=en) interface, enabling users to examine variables, time period, regions etc., and retrieve only the subset they need while the bulk remains in place. Alongside native model-grid resolution, the data is also provided on a common ¼ degree regular grid to facilitate inter-model comparison.  Finally, we employ widely used standards and publish standardized products through established climate-data services (ESGF; https://esgf-metagrid.cloud.dkrz.de/search and WDCC; https://www.wdc-climate.de/ui/project?acronym=EERIE). We also aim to publish the processing scripts used throughout the pipeline, enabling others to build on the lessons learned from the EERIE approach.

How to cite: Wickramage, C., Wachsmann, F., Kröger, J., Ghosh, R., and Aengenheyster, M.: Making Kilometer-Scale Earth System Model (ESM) simulations usable: A workflow approach from European Eddy RIch ESMs (EERIE) project., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19451, https://doi.org/10.5194/egusphere-egu26-19451, 2026.

EGU26-20269 | Posters on site | ESSI2.7

Federated AI-Cubes: Towards Democratizing Big Earth Datacube Analytics 

Peter Baumann, Dimitar Misev, Bang Pham Huu, and Vlad Merticariu

Datacubes are an acknowledged cornerstone for analysis-ready Big Earth Data as they allow more intuitive, powerful services than zillions of "scenes". By abstracting from technical pains they offer two main advantages: for users, it gets more convenient; servers can dynamically optimize, orchestrate, and distribute processing.
We propose a combination of datacube service enhancements which we consider critical for making data exploitation more open to non-experts and more powerful, summarized as "Federated AI-Cubes": 

  • Location-transparent federation allows users and tools to perceive all datacube assets as a single dataspace, making distributed data fusion a commodity. Instrumental for this is automatic data homogenization performed at import and at query time, based on the open Coverage standards.
  • High-level datacube query languages, such as SQL/MDA and ISO/OGC WCPS, simplify analysis and open up data exploitation to non-programmers. Server-side optimization can automatically generate the individually best distributed workflow for every incoming query. At the same time, queries document workflows without low-level technical garbage, making them reproducible. 
  • The seamless integration of AI into datacube analytics plus AI-assisted query writing open up new opportunities for zero-coding exploitation. By not hardwiring a particular model a platform for easy-to-use model sharing emerges. Model Fencing, a new research direction, aims at enabling the server to estimate accuracy of ML model inference embedded in datacube queries. 
  • Standards-based interoperability allows users to remain in the comfort zone of their well-known clients, from map browsing over QGIS and ArcGIS up to openEO, R, and python frontends.
  • Cloud/edge integration opens up opportunities for seamless federation of data centers with moving data sources, such as satellites, including flexible onboard processing.

In summary, these capabilities together have potential for empowering non-experts and making experts more productive, ultimately democratizing Big Earth Data exploitation and widening Open Science.
In our talk, we discuss these techniques based on their implementation in the rasdaman Array DBMS, the pioneer datacube engine, which is operational on multi-Petabyte global assets contributed by research centers in Europe, USA, and Asia. We present challenges and results, supported by live demos many of which are public. Additionally, being editor of the OGC and ISO coverage standards suite, we provide an update on recent progress and future developments.
This research is being co-funded by the European Commission through EFRE projects FAIRgeo and SkyFed.

How to cite: Baumann, P., Misev, D., Pham Huu, B., and Merticariu, V.: Federated AI-Cubes: Towards Democratizing Big Earth Datacube Analytics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20269, https://doi.org/10.5194/egusphere-egu26-20269, 2026.

EGU26-21194 | ECS | Posters on site | ESSI2.7

PHENOMENA: a modular HPC model to facilitate automatic high-resolution greenhouse gas emission monitoring 

Carmen Piñero-Megías, Laura Herrero, Artur Viñas, Johanna Gehlen, Luca Rizza, Ivan Lombardich, Oliver Legarreta, Òscar Collado, Paula Camps, Aina Gaya-Àvila, Marc Guevara, Paula Castesana, and Carles Tena

This work presents the sPanisH EmissioN mOnitoring systeM for grEeNhouse gAses (PHENOMENA), a python-based, open-source, multiscale emission model that computes high resolution (up to 1km2 and daily) and low latency greenhouse gas (GHG) emissions for Spain. The system uses a bottom-up approach, based on emission factors and activity data, and consists of four different modules: First, the downloading module retrieves low latency activity data from multiple sources, including APIs, open data repositories, websites, and private providers, with error handling and automatic retrials to minimize manual intervention. Next, the preprocessing module standardizes the data and applies quality-control checks. The activity data is then combined with emission factors in the calculation module, which covers 11 emission sectors. Finally, the resulting emissions are post-processed to meet the requirements of an open web platform where the results are displayed.

PHENOMENA is based on the OOP paradigm and designed to run on High Performance Computing (HPC) infrastructures. While each one of the emission sectors can run in parallel using MPI strategies, it is still not feasible to run all of them at the same time or download all the activity data at once, as different data providers have different temporal availability. Thanks to the modularity of the system, it can be split into different HPC jobs to handle the heterogeneous data frequencies, increase robustness through automatic retrials, run different instances at the same time and automatize monthly uploads to the web portal, using the Autosubmit workflow manager.

The resulting product is a web app which provides daily 1 km x 1 km gridded emission maps and emission totals aggregated per region and sector. The system's latency is determined by the availability of the activity data from external providers, ranging from daily updates to delays of up to four months.

PHENOMENA allows monitoring low-latency GHG emissions for Spain at high temporal and spatial resolution, providing information in an accessible way to support national to local policymakers. The system is scalable, robust against failures, and easily adaptable to new data providers, regions and emission sectors.

How to cite: Piñero-Megías, C., Herrero, L., Viñas, A., Gehlen, J., Rizza, L., Lombardich, I., Legarreta, O., Collado, Ò., Camps, P., Gaya-Àvila, A., Guevara, M., Castesana, P., and Tena, C.: PHENOMENA: a modular HPC model to facilitate automatic high-resolution greenhouse gas emission monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21194, https://doi.org/10.5194/egusphere-egu26-21194, 2026.

The current era of Earth Observation (EO) is marked by an unprecedented increase in data volume and a growing number of satellite missions, driving a transition from dedicated processing infrastructure to cloud-native, distributed, and scalable orchestration. As Earth System Science, industry, and society increasingly rely on near-real-time EO data, efficient processing and workflow management have become critical components of modern ground segments. This presentation introduces an operational framework designed to meet the challenges of large-scale EO data processing. Examples from the Copernicus Sentinel programme and ESA’s Earth Explorer missions illustrate the framework’s scalable cloud deployment and operational performance. Common challenges - such as handling geospatial data formats, managing ground-segment anomalies, ensuring cybersecurity, providing standardized service interfaces, and leveraging public-cloud infrastructure - are addressed through a unified workflow approach. Operational experience from Copernicus payload data ground segment services, including monitoring via dashboards and control procedures, serves as a model for scientific missions and initiatives adopting these proven concepts. Scalability has emerged as a key feature, enabling efficient data transfers for the Copernicus Long-Term Archive, data access for Copernicus services, and higher-level processing workflows for scientific missions like BIOMASS. These orchestration strategies optimize resource use and energy efficiency for on-demand processing. The generic processing concepts demonstrated in the Copernicus and Earth Explorer programmes offer inspiration for new applications within the Earth System Science community, including hybrid approaches that integrate observations and simulation data.

How to cite: Hofmeister, R.:  A unified framework for large-scale, operational data processing in Earth Observation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21804, https://doi.org/10.5194/egusphere-egu26-21804, 2026.

EGU26-21909 | ECS | Orals | ESSI2.7

Workflow Modernization for Open and Scalable Access to Operational NWP Data 

Nina Burgdorfer, Christian Kanesan, Victoria Cherkas, Noemi Nellen, Carlos Osuna, Katrin Ehlert, and Oliver Fuhrer

Operational Numerical Weather Prediction (NWP) workflows are increasingly challenged by rapidly growing data volumes, expanding product diversity, and the need for timely and scalable access to model data. At the same time, modern Earth system services are evolving toward open data policies that require not only standardized access to model output for internal and external users, but also flexible mechanisms to extract and process relevant information in a FAIR (Findable, Accessible, Interoperable, and Reusable) manner. In this context, MeteoSwiss, in collaboration with the European Centre for Medium-Range Weather Forecasts (ECMWF), is developing a modernized data workflow to improve access to NWP model data for internal and external downstream users. 

The redesigned workflow shifts from a product-centric dissemination model toward a scalable data-as-a-service approach. Rather than relying on the generation and distribution of numerous predefined products, recent ICON forecast output is organized in the Field Database (FDB) and exposed through Polytope, which provides semantic data access and feature extraction capabilities. The workflow automates the ingestion, indexing, access control, and on-demand extraction of forecast fields, and integrates these steps into existing HPC-based production workflows and downstream processing pipelines. By replacing file-based product generation with database-backed access, the workflow enables deterministic data extraction, explicit provenance tracking, and consistent versioning of datasets, so that identical data requests can be reproduced reliably across time and environments. We present recent developments in Earthkit and Polytope that, for the first time, enable such automated workflows on the icosahedral grids used by ICON. Standardized interfaces and modern processing tools from the Earthkit Python ecosystem enable downstream users and applications to retrieve and process tailored subsets of NWP data on demand. 

Our use of open-source, community-developed software (FDB, Polytope, Earthkit) as core workflow components illustrates how ECMWF technologies can be integrated into national weather service environments. Operational experience gained in this context contributes to improving the maturity and usability of these tools and supports their broader adoption by other ECMWF Member States, facilitating the transfer of FAIR, workflow-based data access concepts across the weather and climate community. 

How to cite: Burgdorfer, N., Kanesan, C., Cherkas, V., Nellen, N., Osuna, C., Ehlert, K., and Fuhrer, O.: Workflow Modernization for Open and Scalable Access to Operational NWP Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21909, https://doi.org/10.5194/egusphere-egu26-21909, 2026.

EGU26-22151 | ECS | Posters on site | ESSI2.7

Earthscope Seafloor Geodesy Tools 

Franklyn Dunbar, Mike Gottlieb, Rachel Akie, and David Mencin

Earth System Science increasingly depends on scalable, reproducible computational workflows to manage complex data processing across heterogeneous environments and cloud infrastructure. In seafloor geodesy — a domain where high-resolution geodetic time series and acoustic ranging techniques are essential for understanding submarine tectonic and deformation processes — the need for robust, automated tooling is acute. We present Earthscope Seafloor Geodesy Tools, an open-source Python library developed by Earthscope consortium that supports preprocessing and GNSS-A processing workflows for seafloor geodesy data collected via autonomous wave glider platforms.
Earthscope Seafloor Geodesy Tools, provides modular utilities to translate, organize, validate, and prepare raw observational data for integration with GNSS-A positional solver inversion software (e.g., GARPOS), enabling reproducible, data pipelines within research and operational contexts. By encapsulating domain-specific processing steps into composable components, Earthscope Seafloor Geodesy Tools, enables workflow orchestration and large scale data processing across environments (i.e. local vs remote) and reproducibility of results.

How to cite: Dunbar, F., Gottlieb, M., Akie, R., and Mencin, D.: Earthscope Seafloor Geodesy Tools, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22151, https://doi.org/10.5194/egusphere-egu26-22151, 2026.

GI4 – Earth Observation Systems and Instrumentation

EGU26-1123 | ECS | Posters on site | GI4.2

Deep Learning-Based Hydrometeor Classification from E-Profile Ceilometers Using Cloudnet Reference Data 

Ana del Águila, Anne-Claire Billault-Roux, Eric Sauvageat, Adrián Canella-Ortiz, Laurel Molina-Párraga, Lucas Alados-Arboledas, and Alexander Haefele

Ground-based lidar networks have expanded rapidly in recent years, providing continuous, high-resolution profiles of aerosols, precipitation and clouds for both operational meteorology and climate research. Among them, the EUMETNET E-Profile network now operates more than 400 single-wavelength ceilometers, enabling unprecedented spatial and temporal coverage of backscatter measurements. However, unlike synergistic radar-lidar systems such as Cloudnet, ceilometers alone do not provide operational target classification of hydrometeors or aerosol/clear-sky discrimination.

In this study, we explore the capability of artificial intelligence methods to infer Cloudnet-level target classifications directly from ceilometer backscatter profiles. The approach treats standardized 24-h time-height backscatter as image-like inputs and applies convolutional encoder-decoder architectures for semantic segmentation of atmospheric structures. Training and validation were performed using data from multiple Cloudnet reference stations at different latitudes under diverse meteorological conditions, enabling the model to learn station-agnostic spatio-temporal patterns associated with hydrometeors and aerosol layers.

Initial results demonstrate that key Cloudnet hydrometeor categories and clear-sky/aerosol regions can be recovered from ceilometer-only input, even in the absence of synergistic radar information. These findings indicate that single-wavelength backscatter can be used as input in computer-vision models, in order to extract physically meaningful patterns from the temporal evolution of the signal.

This work establishes the basis for a future near-real-time classification framework scalable to the E-Profile network. The methodology also opens new opportunities for cross-validation with spaceborne lidar and radar products, particularly from the EarthCARE mission, and for generating long-term occurrence statistics that may inform studies on cloud processes, aerosol-cloud interactions and model performance.

Acknowledgements:

This research is part of the Spanish national project PID2023-151817OA-I00, titled DeepAtmo, funded by MICIU/AEI/10.13039/501100011033 and Horizon Europe program under the Marie Sklodowska-Curie Staff Exchange Actions with the project GRASP-SYNERGY (grant agreement No. 101131631). This work is also part of the 2024 Leonardo Grant for Researchers and Cultural Creators from the BBVA Foundation. Ana del Águila is part of Juan de la Cierva programme through grant JDC2022-048231-I funded by MICIU/AEI/10.13039/501100011033 and by European Union “NextGenerationEU”/PRTR.

How to cite: del Águila, A., Billault-Roux, A.-C., Sauvageat, E., Canella-Ortiz, A., Molina-Párraga, L., Alados-Arboledas, L., and Haefele, A.: Deep Learning-Based Hydrometeor Classification from E-Profile Ceilometers Using Cloudnet Reference Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1123, https://doi.org/10.5194/egusphere-egu26-1123, 2026.

EGU26-1153 | ECS | Posters on site | GI4.2

Atmospheric classification using lidar data and deep learning-based image segmentation 

Adrián Canella-Ortiz, Siham Tabik, Sol Fernández-Carvelo, Onel Rodríguez-Navarro, Lucas Alados-Arboledas, and Ana del Águila

Reliable identification of aerosols and clouds in multiwavelength lidar observations remains essential for atmospheric monitoring and climate research. However, conventional processing pipelines rely heavily on expert-driven inversions and threshold-based algorithms. In this work, we present a deep-learning (DL) image segmentation framework designed to operate directly on image-like representations of the range-corrected signal (RCS) and applicable across distinct lidar platforms.

The models were trained on DL4Lidar, a new expert-annotated dataset derived from the ALHAMBRA multi-spectral Raman lidar (Granada, Spain). Using Mask R-CNN implemented using Detectron2 framework, we systematically explored wavelength selection, visualization scale bounds, and architectural variants to maximize the discrimination of atmospheric structures. The resulting class-specific models capture the characteristic morphology and spatiotemporal variability of aerosols and clouds without relying on inversion-based preprocessing, demonstrating the suitability of computer-vision techniques for processing raw lidar observations.

To assess robustness beyond the training instrument, the trained models were directly applied, without retraining or domain adaptation, to measurements from MULHACEN, an independent Raman lidar located in the same facilities as ALHAMBRA but with different hardware characteristics and signal levels. Despite these instrumental differences, the models exhibit stable behavior, correctly identifying cloud and aerosol structures across a wide range of atmospheric situations. This cross-instrument evaluation highlights the capacity of the proposed method to generalize under realistic domain shifts, suggesting that morphological characteristics learned from RCS imagery are transferable across similar ground-based systems.

Experiments and sensitivity analysis of the models will be evaluated for different variables such as attenuated backscatter vs. RCS used as input images. Moreover, the best DL model resulting from the sensitivity analysis will be tested on other lidar instruments within the EARLINET/ACTRIS network and spaceborne observations such as ATLID onboard the EarthCARE mission.

Overall, this work introduces a unified DL-based pipeline for atmospheric structure segmentation from multi-wavelength lidar measurements, demonstrating its potential for operational use and large-scale automated analysis for atmospheric classification across heterogeneous lidar platforms.

Acknowledgements

This research is part of the Spanish national project PID2023-151817OA-I00, titled DeepAtmo, funded by MICIU/AEI/10.13039/501100011033.

How to cite: Canella-Ortiz, A., Tabik, S., Fernández-Carvelo, S., Rodríguez-Navarro, O., Alados-Arboledas, L., and del Águila, A.: Atmospheric classification using lidar data and deep learning-based image segmentation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1153, https://doi.org/10.5194/egusphere-egu26-1153, 2026.

EGU26-2474 | ECS | Posters on site | GI4.2

Machine Learning Reveals Hidden Bias in ERA5 Cloud Heights Over Earth's Third Pole 

Wei Zhao, Yinan Wang, and Yubing Pan

Accurate cloud base height (CBH) over the Tibetan Plateau—Earth's Third Pole—is essential for constraining Asian monsoon dynamics, glacial melt projections, and water security, affecting 1.9 billion people downstream. However, ERA5 reanalysis systematically underestimates CBH by up to 5.20 km in southern regions, propagating errors into climate models and hydrological forecasts. Here, we present a two-step machine learning framework that progressively eliminates this hidden bias. Step 1 refines the ERA5 retrieval algorithm using three years of ground-based lidar observations (October 2021–December 2024), reducing the site-level mean bias error from 1.8 km to 0.1 km and improving the regional correlation with CALIPSO from 0.25 to 0.40. Step 2 applies an Optuna-optimized XGBoost model trained on high-confidence CALIPSO observations (N=106,718), fusing the refined ERA5 data with vertical atmospheric profiles and surface attributes. The final product achieved a test-set RMSE of 1.87 km (R²=0.71, MBE=−0.02 km), with seasonal correlations reaching 0.72–0.86 and southern plateau bias reduced from −5.20 km to −0.11 km, a 97.9% improvement. This scalable approach enables reliable, long-term CBH reconstruction, which is critical for advancing climate model parameterizations and water resource assessments across High Mountain Asia.

How to cite: Zhao, W., Wang, Y., and Pan, Y.: Machine Learning Reveals Hidden Bias in ERA5 Cloud Heights Over Earth's Third Pole, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2474, https://doi.org/10.5194/egusphere-egu26-2474, 2026.

Doppler wind Lidars (DWLs) have been widely used to detect wind vector variations, based on ground monitoring of atmospheric boundary layer and wind shear. This study evaluates the performance between three DWLs and in situ balloon radiosonde. Lidars data comparison focuses on low altitudes (height < 2 km) from July to September 2021 from three producers: MSD (Minshida), CUIT (homemade), and WP (windprofile) Lidars. Within the research height range, comparisons show the root mean square errors (RMSE) for wind speed were 1.11 m s-1, 4.45 m s-1, and 5.15 m s-1, while wind direction RMSE were shown at 49.83°, 82.89°, and 84.87°, respectively. The measurement accuracy decreases with the altitude increase (up to 2km). The Lidar performance requires a certain amount of aerosol backscattering, when PM2.5 ranges within 35-50 µg m-³, MSD Lidar exhibited the highest wind speed correlation (R² = 0.82) with radiosonde, and the wind direction accuracy observed with the three Lidars is enhanced with the increase of aerosol concentration, indicating that particle loading is the critical factor affecting the wind profile. Lidar performance varied significantly with planetary boundary layer heights (PBLH), particularly, the Lidar performance is relatively optimal when the PBLH within 500-750 m, with the Pearson correlation coefficients (PCCs) of wind speed are 0.97, 0.92, and 0.72, while the wind direction is shown at 0.98, 0.75, and 0.70, respectively. The vertical relationship between cloud base height (CBH) and PBLH had also varied influences on the Lidar measurements. Machine learning was used to remove anomalies and complement missing values, the random forest (RF) demonstrated superior performance, with the Area Under the Curve (AUC) of 0.93(CUIT) and 0.90(WP) in the Receiver Operating Characteristic (ROC) curves. RF-based correction of CUIT data enhanced the R² from 0.42 to 0.65. The R² between the RF-based CUIT and Aeolus satellite data was 0.83, indicating that the method effectively improved data, even in circumstances of anomalies. We proposed a new correction algorithm combined with the isolation forest (IF) and RF to handle high-dimensional and incomplete datasets. Our procedure could increase the Lidar measurement quality of wind.

How to cite: Zhang, Y., Hu, H., Luo, J., and Wu, H.: Comparison of the Performance between Three Doppler wind Lidars and a Novel Wind Speed Correction Algorithm, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4831, https://doi.org/10.5194/egusphere-egu26-4831, 2026.

EGU26-5579 | Orals | GI4.2

Water Vapor DIAL in Space: Which Performance Should you Expect? 

Martin Wirth and Silke Groß

Water vapor is the key trace gas component of the air and involved in virtually all relevant atmospheric processes. To know the vertical profile with decent resolution is crucial in all cases. For example, there are several regions of the atmosphere where numerical weather prediction models show biases which are not understood. And recent studies have shown that the boundary layer moisture and isolated lofted humidity layers play a key role in the initiation of convection.  So, after aerosol/cloud and wind lidars have been very successfully applied within space missions, the natural next step would be the profiling of water vapor by a Differential Absorption Lidar (DIAL) from a satellite on a low Earth orbit. Thanks to the European spaceborne lidar missions Aeolus/2, EarthCARE, and MERLIN now the major building blocks for such a water vapor DIAL have reached the necessary technological readiness and the last open issue, a high-power laser source at 935 nm, is currently addressed by an ESA project.

A key tool to assess the impact of certain design decisions on the performance is a full end-to-end simulation tool. DLR has developed and kept up to date such a tool over the past years. In our presentation we will show the achievable resolution and precision of a spaceborne H2O-DIAL in dependence of key design parameters like number of wavelengths, laser power, telescope diameter and detector noise for several real-world atmospheric scenes that have been captured with our airborne demonstrator. Special focus will be given to non-standard profile situations where especially passive sounding systems have difficulties due to their limited vertical resolution. This presentation is thought as a starting point for further discussions with potential users of data from a space-borne H2O-DIAL to refine the observational requirements and adjust the lidar-parameters on the system level.

How to cite: Wirth, M. and Groß, S.: Water Vapor DIAL in Space: Which Performance Should you Expect?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5579, https://doi.org/10.5194/egusphere-egu26-5579, 2026.

EGU26-5843 | Posters on site | GI4.2

The space lidar mission LUCE: a multi-disciplinary observatory for Earth Sciences 

Paolo Di Girolamo and the LUCE

LUCE, formerly Cloud and Aerosol Lidar for Global Scale Observations of the Ocean-Land-Atmosphere System (CALIGOLA), is an advanced multi-disciplinary space lidar mission for Earth Sciences, primarily focusing on the observation of the atmosphere and oceans, aimed at advancing global knowledge on the coupled atmosphere-ocean-land system. It is the first spaceborne Raman-elastic-fluorescence lidar, created through an Agenzia Spaziale Italiana (ASI) and National Aeronautics and Space Administration (NASA) partnership. This mission has been conceived with the aim to provide the international scientific community with an unprecedented dataset of geophysical parameters capable to increase scientific knowledge in the areas of atmospheric, aquatic, terrestrial, cryospheric and hydrological sciences. The mission is planned to be launched in the time frame 2035-2037, with an expected lifetime of 3-5 years. This conference contribution aims at providing an overview of the different mission scientific objectives, with a primary focus on atmospheric and ocean sciences, and a preliminary assessment of the expected system performance in a variety of environmental scenarios.

How to cite: Di Girolamo, P. and the LUCE: The space lidar mission LUCE: a multi-disciplinary observatory for Earth Sciences, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5843, https://doi.org/10.5194/egusphere-egu26-5843, 2026.

EGU26-6439 | Orals | GI4.2

Planetary Boundary Layer Height and Air Quality during Heatwaves in contrasting climate regions from CALIPSO lidar retrievals. 

Simone Lolli, Andreu Salcedo-Bosch, Francesc Rocadenbosch, Carina Argañaraz, Gabriele Curci, and Yuanjian Yang

The Height of the Planetary Boundary Layer (PBLH) plays a key role in controlling how air pollutants accumulate and disperse during heatwaves, yet its large-scale behaviour across different climate regimes remains poorly understood. In this study, we use a 10-year PBLH dataset derived from CALIPSO CALIOP Level-1 backscatter data, retrieved with a Random Forest model trained on radiosonde-based PBLH observations, to investigate boundary-layer dynamics during heatwaves across several regions of the world. The resulting product provides PBLH estimates at approximately 20 × 20 km resolution and shows good performance in mid-latitude regions under a wide range of aerosol and cloud conditions.

Heatwaves are identified using ERA5 daily maximum temperature anomalies, applying region-specific percentile and persistence criteria over the Mediterranean and central Europe, the United States, eastern China megacities, and selected arid–subtropical areas. For each region, we construct composites of the diurnal evolution of PBLH during heatwave and non-heatwave summers and relate them to co-located surface PM2.5 and ozone observations from air-quality monitoring networks. This approach allows us to quantify regional differences in PBLH anomalies and in the sensitivity of PM2.5 and ozone to PBLH variations during heatwaves. We also examine how different stages of the heatwave life cycle are reflected in PBL evolution and the persistence of residual layers, highlighting implications for compound heatwave–air-pollution risks in a warming climate.

How to cite: Lolli, S., Salcedo-Bosch, A., Rocadenbosch, F., Argañaraz, C., Curci, G., and Yang, Y.: Planetary Boundary Layer Height and Air Quality during Heatwaves in contrasting climate regions from CALIPSO lidar retrievals., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6439, https://doi.org/10.5194/egusphere-egu26-6439, 2026.

EGU26-7182 | Orals | GI4.2

Long-term (2010-2024) lidar observations of cirrus clouds at Wuhan (30.5°N, 114.4°E), China 

Yun He, Tingyang Fu, Zhenping Yin, Weijie Zou, Dongzhe Jing, Fan Yi, and Longlong Wang

Cirrus clouds play a crucial role in the Earth’s climate by regulating its radiative balance. Their optical and radiative properties exhibit significant variability, influenced by both spatial and temporal distribution. This study investigates the geometrical and optical properties of cirrus clouds using 15 years (2010–2024) of 532-nm ground-based polarization lidar observations at Wuhan (30.5°N, 114.4°E), a mid-latitude site over central China. A cloud detection algorithm and optical parameter inversion procedure were developed to identify overall 2033 cirrus cases. The geometrical and optical characteristics of these clouds were analyzed in detail. Cirrus clouds have cloud top and base heights of 12.4±2.1 km and 9.7±2.6 km, respectively, with thickness of 2.7±1.6 km and cloud top temperature of -50.2 ± 9.0 °C. Cloud top height reaches its maximum in summer (13.8 km) and minimum in winter (9.6 km). The cloud optical depth is variable, mainly ranging from 0 to 1 with an average of 0.34±0.35, suggesting that cirrus clouds are predominantly optically thin to moderately thick. The lidar ratio is 28.58±12.57 sr, while the volume and particle depolarization ratios are 0.32±0.08 and 0.40±0.11, respectively. These findings generally reflect the typical characteristics of cirrus clouds in the Asian mid-latitude region.

How to cite: He, Y., Fu, T., Yin, Z., Zou, W., Jing, D., Yi, F., and Wang, L.: Long-term (2010-2024) lidar observations of cirrus clouds at Wuhan (30.5°N, 114.4°E), China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7182, https://doi.org/10.5194/egusphere-egu26-7182, 2026.

EGU26-7551 | Orals | GI4.2

MERLIN laser transmitter - Laser performance for critical mission objectives and outlook for future missions 

Jana Ammersbach, Heinrich Faidel, Martin Giesberts, Bastian Gronloh, Tristan Heider, Hans-Dieter Hoffmann, Jörg Luttmann, Melina Reiter, Rolf Versteeg, and Matthias Winzen

The Methane Remote Sensing LiDAR Mission (MERLIN) is a Franco-German cooperation between the French Space Agency CNES and the German Space Agency at DLR.

The Laser Optical Bench for the IPDA LiDAR instrument is currently being built at Fraunhofer Institute for Laser Technology, based in Aachen, Germany. The laser bench is one of the core parts of the payload, for which Airbus Defence and Space GmbH is the Prime Contractor. The laser and laser housing design were developed and optimized in close cooperation between Airbus Defence and Space GmbH and Fraunhofer Institute for Laser Technology.

This presentation will provide an overview of the flight hardware’s assembly, integration and test status, the qualification status of all optical components and the lifetime test results for critical components. Furthermore, we will highlight the inherent stability aspects of the laser: for example, the demonstrated stable and full-performance operation of the oscillator and the amplifier over a wide range of thermal boundary conditions. Currently, the last optical stage of the laser, the pre-assembled and fully aligned optical Parametric Oscillator (OPO) is being integrated on the flight laser bench. The qualification module is already completely optically integrated. In the frame of the presentation, we will be showcasing current optical performance of the laser transmitter for flight and qualification module. Additionally, we will provide an outlook on future LiDAR laser concepts based on the developments within the MERLIN project.

How to cite: Ammersbach, J., Faidel, H., Giesberts, M., Gronloh, B., Heider, T., Hoffmann, H.-D., Luttmann, J., Reiter, M., Versteeg, R., and Winzen, M.: MERLIN laser transmitter - Laser performance for critical mission objectives and outlook for future missions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7551, https://doi.org/10.5194/egusphere-egu26-7551, 2026.

EGU26-8018 | ECS | Orals | GI4.2

Long-term analysis of Raman lidar water vapour profiles over the ACTRIS AGORA Granada station 

Arlett Díaz Zurita, Víctor Manuel Naval Hernández, David N. Whiteman, Onel Rodríguez Navarro, Jorge Andrés Muñiz Rosado, Daniel Pérez Ramírez, Lucas Alados Arboledas, and Francisco Navas Guzmán

Water vapour is a crucial and highly variable greenhouse gas in the Earth's atmosphere that plays a major role in the radiative balance, energy transport and photochemical processes. It can also affect the radiative budget indirectly through cloud formation and by altering the size, shape, and chemical composition of aerosol particles. Moreover, monitoring water vapour remains challenging due to its high temporal and spatial variability. Consequently, systematic and accurate observations of water vapour are essential to improve our understanding of its role at both local and global scales and for enhancing climate projections.

Advances in remote sensing techniques have enabled continuous acquisition of precipitable water vapour (PWV) measurements using sun/star photometry, microwave radiometry and the Global Navigation Satellite System (GNSS). Nevertheless, none of these instruments provides information on the vertical distribution of water vapour, a critical information considering that water vapour concentrations typically vary by up to three orders of magnitude between the surface and the upper troposphere. In this context, Raman lidar has demonstrated its ability to capture the spatial and temporal evolution of water vapour in the troposphere. Accurate retrievals of the water vapour mixing ratio from Raman lidar measurements rely on robust and well-characterised calibration procedures as well as on an accurate estimation of the differential atmospheric transmission term, which accounts for extinction differences between the molecular reference (nitrogen and oxygen) and water vapour wavelengths.

In this study, the lidar calibration constant was determined using a hybrid calibration method, which combines correlative PWV measurements for lidar calibration with Numerical Weather Prediction (NWP) data to reconstruct the water vapour profile within the incomplete overlap region of the lidar system. The differential transmission was estimated using an automated method to account for the aerosol contribution, based on sun photometer Aerosol Optical Depth (AOD) measurements and an exponential decay function with attitude to model aerosol extinction (Díaz-Zurita et al., 2025). Subsequently, a long-term database of water vapour profiles over the period 2009-2022 was generated, providing high vertical and temporal resolution measurements of water vapour over the city of Granada, in Southern Spain. A comprehensive statistical analysis was conducted to characterise the vertical distribution of water vapour over a 14-year period, representing the first long-term vertical characterisation of water vapour in this region. Mean interannual and seasonal water vapour profiles were derived for the entire study period, and trend analyses were performed to assess long-term variations in water vapour content in the lower troposphere. Additionally, lidar-derived PWV values were compared with those obtained from microwave radiometer and GNSS observations.

This research was funded by Grant PID2021-128008OB-I00 funded by MICIU/AEI/ 10.13039/501100011033 by ERDF/EU European Union, and by the Spanish national projects CNS2023-145435, PID2023-151817OA-I00 and Marie Skłodowska-Curie Staff Exchange Actions with the project GRASP-SYNERGY (grant agreement no. 10113163).

 

Diaz-Zurita et al. (2025).  Remote Sens. 2025, 17(20), 3444; https://doi.org/10.3390/rs17203444

How to cite: Díaz Zurita, A., Naval Hernández, V. M., Whiteman, D. N., Rodríguez Navarro, O., Muñiz Rosado, J. A., Pérez Ramírez, D., Alados Arboledas, L., and Navas Guzmán, F.: Long-term analysis of Raman lidar water vapour profiles over the ACTRIS AGORA Granada station, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8018, https://doi.org/10.5194/egusphere-egu26-8018, 2026.

EGU26-8349 | ECS | Orals | GI4.2

Ground Based Demonstration of an Airborne High Spectral Resolution Temperature Profiling Lidar 

Madison Hetlage, Johnathan Hair, Taylor Shingler, David Harper, and Amin Nehrir

There is a strong desire for improved airborne thermodynamic profiling capabilities, particularly within the planetary boundary layer. While active temperature profiling lidars using rotational Raman scattering and differential oxygen absorption (DIAL) exist for ground-based use, these techniques are limited by the inefficiency of Raman scattering and oxygen DIAL’s need for collocated water vapor and aerosol measurements. This work aims to investigate the sensitivities and signal-to-noise of a temperature high spectral resolution lidar (HSRL) measurement approach for airborne tropospheric temperature profiling and add this capability to the NASA LaRC first generation airborne aerosol and profiling instrument, HSRL-1.

The temperature HSRL technique relies on the thermally sensitive Doppler broadening of the Rayleigh scattering signal. In an aerosol HSRL, a spectral notch filter is used to differentiate between molecular and aerosol backscattering. The addition of a second molecular channel (using a second notch filter with a distinct transmission spectrum) enables an observation dependent on the molecular scattering spectral lineshape (i.e. temperature and pressure) and independent of aerosol scattering. The implementation of an additional channel to the HSRL-1 instrument leverages the current HSRL-1 instrument and data acquisition infrastructure, particularly the flight-tested Nd:YVO4 laser, receiver, and detectors, and exploits the strong signal strength of elastic scattering, resulting in a measurement well suited for the moving, airborne platform.

This presentation will cover the temperature HSRL retrieval technique and discuss the theoretical optimization and experimental characterization of the required HSRL-1 system modifications. The reconfigured system has been operated in a ground-based, zenith-pointing configuration to test the new thermal profiling capability. A set of these results will be examined and compared to co-located radiosonde measurements. Additionally, the expected airborne performance, which has been simulated using signal levels from previous HSRL-1 field deployments, will be presented.

How to cite: Hetlage, M., Hair, J., Shingler, T., Harper, D., and Nehrir, A.: Ground Based Demonstration of an Airborne High Spectral Resolution Temperature Profiling Lidar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8349, https://doi.org/10.5194/egusphere-egu26-8349, 2026.

EGU26-8670 | ECS | Posters on site | GI4.2

AecroFormer: Fast, Noise-Robust Aerosol Microphysical Retrieval for Multiwavelength Raman Lidar 

Weijie Zou, Zhenping Yin, Zhichao Bu, Xuan Wang, and Detlef Müller

Aerosol microphysical parameters (e.g., size distributions and complex refractive index) control scattering and absorption and underpin quantitative estimates of aerosol radiative effects and aerosol–cloud interactions. Retrieving them from multiwavelength Raman lidar is inherently ill-posed: measurement noise and systematic uncertainties quickly erode multi-channel constraints under weak signals, and conventional LUT/iterative inversions are too slow (seconds to minutes per profile) for network-scale or high-throughput processing.

We propose AecroFormer, an end-to-end regression model that incorporates multi-head attention to learn cross-wavelength coupling and deliver physically coherent, range-resolved vertical-profile retrievals with improved stability under real-world SNR and noise. For channel combinations such as 3β+2α, AecroFormer achieves an inference speed of 7.4×10⁻⁵ s per range gate on an NVIDIA GeForce RTX 5080, delivering orders-of-magnitude acceleration relative to LUT/iterative schemes that typically operate from minute-level down to sub-second per range gate (e.g., Müller et al., 1999; Wang et al., 2022). Noise robustness tests show that the model maintains practical accuracy as noise increases: even at 20% noise, it remains stable with MAE(mᵣ) ≈ 0.0758 and MRE(rₑ) ≈ 32.9%.

Focusing on the two important application-critical profile products—effective radius (rₑ) and aerosol volume concentration—we assessed real-world applicability through  an observation-based consistency check using operational measurements from the Aksu site (Xinjiang, China) in January 2024, selecting four days for validation. Retrieved aerosol volume concentrations were converted to 0–2 km boundary-layer mean PM₂.₅ using an empirical density assumption and matched against surface air-quality observations (n = 28). The comparison yields a PM₂.₅ bias of 4.69 ± 26.87 µg/m³ and a relative bias of 3.29%, indicating that the method reproduces both the magnitude and variability observed by ground monitoring in a network-operational setting.

Overall, AecroFormer substantially reduces the computational cost while preserving noise-robust retrieval performance, enabling a practical transition from offline, slow microphysical inversions to near-real-time, high-throughput, and deployable processing. It also provides a reusable algorithmic foundation for future extensions under more realistic bimodal forward assumptions and tightly controlled uncertainty constraints.

How to cite: Zou, W., Yin, Z., Bu, Z., Wang, X., and Müller, D.: AecroFormer: Fast, Noise-Robust Aerosol Microphysical Retrieval for Multiwavelength Raman Lidar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8670, https://doi.org/10.5194/egusphere-egu26-8670, 2026.

Accurately understanding the vertical distribution of major global atmospheric gases is a critical issue in climate change research and response. The  Low Earth Orbit-to-Low Earth Orbit (LEO-LEO) infrared laser occultation (LIO) detection technology enables three-dimensional, all-time, and high vertical-resolution simultaneous detection of multiple atmospheric composition (CO2, CH4, H2O, O3, N2O, CO, etc.) and line-of-sight wind speed. This approach is expected to complement existing greenhouse gas column total measurement methods in the future. The LIO system consists of a transmitter and a receiver. It employs eleven carefully selected infrared laser signals within the shortwave infrared (SWIR) spectral region of 2–2.5 µm. Based on the differential absorption lidar (DIAL) principle, the system retrieves vertical profiles of greenhouse gases and further derives line-of-sight wind speed via spectral Doppler frequency shift. During an occultation event, the laser signal emitted by the transmitter is attenuated by the atmosphere before reaching the receiver. The transmitter realizes differential absorption atmospheric spectral detection through multiple laser channels. Each detection element adopts dual-channel detection, and the receiver performs high-sensitivity detection for each spectral channel. To ensure precise laser wavelength control, the LIO system adopts optical frequency comb stabilization technology. Additionally, a spatial heterodyne spectrometer is used to achieve extremely high spectral resolution within a narrow field of view. By scanning the Earth's atmosphere from top to bottom, the system allows for high-precision retrieval of trace gases profiles. Currently, no LEO-LEO occultation mission has been deployed in space. Research has been focused on frequency selection evaluation, inversion algorithm refinement, occultation orbit design, and detection performance simulations. The continued development of infrared laser occultation technology can provide essential vertical atmospheric datasets for future global climate change research.

How to cite: Wang, X., Zhang, Z., and Zong, X.: Advances in Space-borne Infrared Laser Occultation for Atmospheric Composition Profiles Detection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10217, https://doi.org/10.5194/egusphere-egu26-10217, 2026.

A wide range of weather phenomena, including for example valley circulations and convective initiation, are connected to mesoscale wind fluctuations. Their representation in convective-scale numerical weather prediction models, particularly in complex terrain, remains uncertain but may significantly affect forecast quality.
To quantify the potential added value of denser wind observation networks, we assimilate 3 months of data from a network of 12 Doppler wind lidars obtained during the Swabian MOSES campaign around the Black Forest region in southwestern Germany during summer 2023. Vertical profiles of the horizontal wind components up to approximately 4 km altitude retrieved from the wind lidars were assimilated using the regional forecasting system of the German Weather Service based on the Kilometer-Scale Ensemble Data Assimilation (KENDA) system using a Local Ensemble Transform Kalman Filter (LETKF) and the ICOsahedral Non-hydrostatic (ICON) model.Overall, ICON represents the wind fields well and the assimilation reduces short-term forecast errors. As expected, the observation influence is largest within the campaign region but also spreads horizontally and vertically away from it. Differences between observations and model tend to be particularly large during convective conditions. Moreover, assimilating the dense wind information leads to small but systematic differences in wind speed and direction compared to an experiment without Doppler wind lidar assimilation. On average, the zonal wind speed is slightly overestimated in the model, while the meridional wind speed is underestimated, resulting in a rotation of the wind direction. The underlying causes of this bias are currently under investigation.

How to cite: Oertel, A., Thomas, J., Reich, H., Keller, J., and Knippertz, P.: The influence of assimilating Doppler wind lidar observations from the Swabian MOSES 2023 campaign on mesoscale wind variability over southwestern Germany, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10835, https://doi.org/10.5194/egusphere-egu26-10835, 2026.

Wildfire activities across Canada have increased significantly in the last several years. Intense wildfires release large amounts of smoke aerosols that can be lifted into the upper troposphere and lower stratosphere, providing a large episodic source of carbonaceous aerosols, composed primarily of organic carbon and black carbon. These smoke particles can persist for weeks to months and be transported over long distances, whereby extending their atmospheric influence far from the source regions. Smoke particles can greatly impact the Earth’s climate directly by scattering and absorbing solar radiation and indirectly by modifying cloud formation and properties. During long-range transport, smoke aerosols undergo chemical and microphysical aging, which may alter their size, composition, optical properties, and ice nucleation ability. In addition, smoke particles in the high altitudes can act as ice-nucleating particles (INP) to trigger cirrus cloud formation via heteorogeneous nucleation, modifying ice crystal number concnetrations, particle size and cloud optical properties. From the end of May 2025, extreme wildfire outbreak in Canada lifted smoke particles up to the lower stratosphere that were transported across the North Atlantic to Europe. In this study, we paramerize the aging transformations of smoke aerosols by comparing their lidar ratios (= extinction-to-backscatter ratio) and particle linear depolarization ratios (PLDR) directly retrieved by ATLID (the ATmospheric LIDar) onboard the EarthCARE satellite along the transport pathway of the smoke plumes. To do so, we make use of the HYSPLIT forward trajectories to track the smoke plume evolving from fire locations. Furthermore, we derive the cirrus cloud PLDR from ATLID as well as ice crystal number concentration (Ni) and effective radius (Re) from the lidar-radar synergy combing co-located ATLID and CPR (the Cloud Profiling Radar). Finally, we are able to compare PLDR, Ni, and Re between disturbed cirrus clouds by smoke aerosols and pristine ones to identify the impact of smoke particles on cirrus clouds. 

How to cite: Li, Q. and Gross, S.: Aerosol aging and cirrus cloud modification from Canadian wildfire smoke transported to Europe in 2025 observed by EarthCARE, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11060, https://doi.org/10.5194/egusphere-egu26-11060, 2026.

Aerosols play a key role in air quality, weather, and climate. Ground-based active remote sensing can contribute to the continuous monitoring of aerosol vertical profiles, especially when operating within regional, national and international networks. In fact, networked Automated-Lidar-Ceilometers (ALC) are now widely used to this purpose, monitoring the low and middle troposphere. However, conversion of their raw data into quantitative geophysical information is not straightforward.

In this work, we present a model-supported approach to retrieve vertically-resolved aerosol optical and physical properties (aerosol backscatter and extinction coefficients, surface area, volume and mass concentrations) from elastic lidar systems. It extends previous results and processing capabilities of lidar and/or ALC data developed and employed within the Italian ALC network ALICENET (Dionisi et al., 2018; Bellini et al., 2024). In particular, we present here an upgraded version of the model, which relies on a Monte Carlo framework generating a large ensemble of light-scattering computations at multiple, lidar-relevant wavelengths (355, 532, 910, and 1064 nm) and targeted to reproduce a continental aerosol type mixed to low-to-moderate contributions of desert dust. With respect to previous model configurations (e.g., Dionisi et al., 2018), the new version simulate the coarse, dust particles as spheroids, taking advantage of the open-access spheroid package GRASP (Dubovik et al., 2006). This also allows computation of the aerosol depolarization ratio in addition to the other aerosol optical and physical properties. The model simulations are then used to derive mean functional relationships linking aerosol backscatter and particle depolarization ratio to the other aerosol properties. This upgraded version of the model was indeed developed within ALICENET to assist inversion of new commercially available ALC systems with polarization capability (PLC, as the Vaisala CL61). In this work, we will present: a) the numerical model simulations results, b) their evaluation through independent aerosol data from AERONET sun-photometers and 3) their practical use within the operative ALICENET inversion of PLC data to derive aerosol optical and physical properties. In fact, application of the new functional relationships shows improved agreement of PLC-retrievals with columnar aerosol optical depth and in situ mass measured at ground level in dust-loaded conditions. These results suggest that the proposed methodology could be applied to operational ALC/PLC networks operating in low-to-moderate dust-affected conditions, thus supporting radiative transfer, atmospheric chemistry, and air quality studies.

References:

  • Dionisi, et al., A multiwavelength numerical model in support of quantitative retrievals of aerosol properties from automated lidar ceilometers and test applications for AOT and PM10 estimation, Atmos. Meas. Tech., 11, 6013–6042, https://doi.org/10.5194/amt-11-6013-2018, 2018.
  • Bellini, et al., ALICENET– an Italian network of automated lidar ceilometers for four-dimensional aerosol monitoring: infrastructure, data processing, and applications, Atmos. Meas. Tech., 17, 6119–6144, https://doi.org/10.5194/amt 17-6119-2024, 2024.
  • Dubovik et al., Application of spheroid models to account for aerosol particle nonsphericity in remote sensing of desert dust, J. Geophys. Res., 111, D11208, https://doi.org/10.1029/2005JD006619, 2006.

How to cite: Goi, A., Diémoz, H., Bellini, A., Bracci, A., and Barnaba, F.: Model-assisted retrievals of aerosol properties from Polarization-sensitive Automated Lidar-Ceilometers and test applications to Vaisala CL61 measurements during desert dust transport episodes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11591, https://doi.org/10.5194/egusphere-egu26-11591, 2026.

EGU26-12298 | Posters on site | GI4.2

Studying differences in microphysics of ice clouds in the Arctic depending on airmass origin using lidar-radar synergy 

Silke Gross, Georgios Dekoutsidis, Martin Wirth, and Florian Ewald

The climate in the Arctic is changing rapidly. The near-surface air temperature increased much faster than on global average in recent years, a phenomenon called Arctic Amplification. This Arctic Amplification leads to a weaker and wavier jet stream, potentially allowing a more frequent transport of airmasses into the Arctic which have their origin in the mid-latitude. These mid-latitude airmasses are responsible for an influx of warm and moist air, significantly influencing the energy budget in the Arctic due to their radiative effects. But airmass transport from the mid-latitudes has also an impact on cloudiness in the Arctic as well as on cloud properties, as they strongly depend on the conditions under which the clouds form. The main focus on cloud so far, however, was on lower-level clouds. Arctic high level ice clouds are hard to study. Satellite measurements do often not provide data with sufficient accuracy or resolution, and in-situ measurement have rarely been performed.

 

In March and April 2022, the HALO-(AC)3 campaign was conducted, using the German High Altitude and LOnge range (HALO) research aircraft equipped with a remote sensing payload. With HALO it was possible to perform high altitude measurements deep inside the Arctic. The measurements provided high accurate and highly resolved information about the atmosphere along the flight path. Key instruments during HALO-(AC)3 have been the combined airborne water vapor differential absorption and high spectral resolution lidar WALES, and the Doppler cloud radar MIRA-35. We use the measurements of the lidar to characterize the environmental conditions in Arctic and mid-latitude airmasses, i.e. the humidity field. Ice cloud microphysical properties are derived from the synergy of lidar and radar using an optimal estimate retrieval. The combination of the characterization of the environmental conditions and the cloud properties allows to study differences in the microphysics of ice clouds in the Arctic depending on the origin of the airmasses they are forming in. We will give an overview of our measurements, the characterization of the environmental conditions, and will show differences in the cloud macro- and microphysical properties of the observed ice clouds.

How to cite: Gross, S., Dekoutsidis, G., Wirth, M., and Ewald, F.: Studying differences in microphysics of ice clouds in the Arctic depending on airmass origin using lidar-radar synergy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12298, https://doi.org/10.5194/egusphere-egu26-12298, 2026.

EGU26-12789 | ECS | Posters on site | GI4.2

CO2 Profiling with Automated Scanning Raman Lidar 

Moritz Schumacher, Diego Lange, Andreas Behrendt, and Volker Wulfmeyer

Carbon dioxide is the most important anthropogenic greenhouse gas. Therefore, measuring its distribution and variability in the atmosphere with high precision, accuracy, and resolution is key to a better understanding of the carbon cycle and radiative forcing. Especially, continuous profiling at the same location over longer periods of time provides insights about local sources and sinks. Since most of these are located on the ground, ground-based lidar systems with their ability of range-resolved measurements are particularly interesting because passive remote sensing satellites (e.g. OCO-2/3) cannot provide range-resolved data close to the surface. To realize carbon dioxide measurements, we integrated an additional channel into our eye-safe, fully automated ground-based Raman lidar ARTHUS (Atmospheric Raman Temperature and HUmidity Sounder) [1]. So far, more than 90 nights of CO2 profiles have been collected at the Land-Atmosphere Feedback Observatory (LAFO) of the University of Hohenheim, Stuttgart, Germany [2]. Profiles of CO2, temperature, and humidity, as well as particle extinction and particle backscatter coefficients, are measured simultaneously with five receiver channels. With averaging of 1 h and 400 m under nocturnal, cloud-free conditions, the uncertainties of the CO2 mixing ratio measurements are only <2.8 ppm up to a distance of 2 km . When averaging over the full night, e.g., 13 hours and 400 m, the uncertainties are <1 and <2 ppm up to distances of ~2.5 and 4.0 km, respectively. Compared to measurements presented at last year’s EGU General Assembly [3], the lidar CO2 signal intensity could be improved by a factor of up to 8.

Since 2025, a newly installed two-mirror scanner enables measurements in any direction. In December 2025, we performed measurements with an elevation angle of 2° close to the surface in order to investigate CO2 sources and sinks. Furthermore, nearby in-situ CO₂ sensors on towers at 2 and 10 m height above ground at distances of 600 and 1000 m to the lidar now allow for improved calibration and comparisons. We will present and discuss these new low-level scans at the conference.

 

References:

[1] Lange, D. et al.: Compact Operational Tropospheric Water Vapor and Temperature Raman Lidar with Turbulence Resolution. Geophys. Res. Lett. (2019). DOI: 10.1029/2019GL085774

[2] Späth, F., et al.: The land–atmosphere feedback observatory: a new observational approach for characterizing land–atmosphere feedback. Geoscientific Instrumentation, Methods and Data Systems (2023). DOI: 10.5194/gi-12-25-2023

[3] Schumacher, M., D. Lange, A. Behrendt, V. Wulfmeyer: CO2 Measurements with Raman Lidar in the Lower Troposphere. EGU25-8872 (2025) DOI: 10.5194/egusphere-egu25-8872

How to cite: Schumacher, M., Lange, D., Behrendt, A., and Wulfmeyer, V.: CO2 Profiling with Automated Scanning Raman Lidar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12789, https://doi.org/10.5194/egusphere-egu26-12789, 2026.

EGU26-13239 | Posters on site | GI4.2

Studying Land-Atmosphere Feedback Processes With a Synergy of Six Scanning Lidars 

Andreas Behrendt, Moritz Schumacher, Diego Lange, Linus von Klitzing, Syed Abbas, Oliver Branch, Matthias Mauder, and Volker Wulfmeyer

We will present the strategy and results of a combination of six scanning lidars to investigate the interplay between daytime surface fluxes, surface layer gradients, convective boundary layer dynamics and development, as well as the characteristics of the interfacial layer and the lower free troposphere. Our observations were made above the agricultural fields of University of Hohenheim [1], Stuttgart, Germany in spring and summer 2025 in the frame of the research unit Land Atmosphere Feedback Initiative (LAFI, https://lafi-dfg.de/) of the German Research Foundation (DFG). For this, the automated Raman lidar ARTHUS (Atmospheric Temperature and Humidity Sounder) built in our institute in recent years, was extended with a scanner for atmospheric measurements in the surface layer just above the canopy. ARTHUS [2] is an eye-safe rotational Raman lidar with five receiver channels detecting the elastic backscatter signal at 355 nm, two rotational Raman signals with opposite temperature dependence, as well as the two vibrational Raman signals of water vapor and carbon dioxide. These scanning measurements were performed during intensive observation periods for 50 minutes of each hour while during the remaining 10 minutes of each hour as well as during non-IOP days vertical pointing measurements were made. These surface layer observations of ARTHUS were combined with data measured with two Doppler lidars making simultaneously cross-cutting low-level scans for horizontal wind profiling near the surface. Two more Doppler lidars were measuring vertical wind fluctuations and horizontal wind speed and direction. One of these two Doppler lidars was operated in constant vertical pointing mode while the other was operated in a six-beam scanning mode with an elevation angle of 45°. Our water vapor differential absorption lidar (WVDIAL) made vertical-pointing observations of turbulent moisture fluctuations up to the free troposphere. The WVDIAL uses a Titanium-Saphire laser pumped with the second-harmonic radiation of a Nd:YAG laser as transmitter emitting online and offline laser pulses near 820 nm with 200 Hz into the atmosphere. The atmospheric backscatter signals are collected with a 80-cm telescope. While also the WVDIAL can scan in any direction, it was operated in constant vertical-pointing mode during LAFI.

 

[1]        Späth, F., et al.: The land–atmosphere feedback observatory: a new observational approach for characterizing land–atmosphere feedback. Geoscientific Instrumentation, Methods and Data Systems (2023). DOI: 10.5194/gi-12-25-2023

[2]        Lange, D. et al.: Compact Operational Tropospheric Water Vapor and Temperature Raman Lidar with Turbulence Resolution. Geophys. Res. Lett. (2019). DOI: 10.1029/2019GL085774

How to cite: Behrendt, A., Schumacher, M., Lange, D., von Klitzing, L., Abbas, S., Branch, O., Mauder, M., and Wulfmeyer, V.: Studying Land-Atmosphere Feedback Processes With a Synergy of Six Scanning Lidars, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13239, https://doi.org/10.5194/egusphere-egu26-13239, 2026.

EGU26-14184 | Orals | GI4.2

Vertical profiling of aerosol optical, microphysical, and chemical properties using elastic-Raman-LIF lidars and in situ aerosol measurements during the 2024–2025 CHOPIN campaign 

Alexandros D. Papayannis, Marilena Gidarakou, Nikos Kafenidis, Igor Veselovskii, Romanos Foskinis, Olga Zografou, Maria I. Gini, Konstantinos Granakis, Paul Zieger, Aiden Jonsson, Julia Schmale, Konstantinos Eleftheriadis, and Athanasios Nenes

The Cleancloud Helmos OrograPhic site experimeNt (CHOPIN) campaign took place at mount Helmos, Greece (37.98°N, 22.2°E; 1700-2314 m a.s.l.) to  study the aerosol-cloud interactions during two distinct periods: autumn/winter (October–November 2024) and spring (April–May 2025). In situ aerosol sampling at the Helmos Atmospheric Aerosol and Climate Change Station (HAC)2 was performed at 2314 m a.s.l. along with aerosol lidar vertical measurements. (HAC)2 is located on a strategic site at a crossroad of different air masses containing various aerosol types (wildfire smoke, mineral dust, continental pollution, marine aerosols, and biogenic particles). Two lidar systems were deployed: the AIAS depolarization lidar (532 nm parallel and cross, 1064 nm) and the ATLAS-NEF multi-wavelength elastic-Raman-LIF lidar (355, 387, 407 and 420-520 nm). The vertically resolved aerosol optical properties (extinction and backscatter coefficient, lidar ratio, Ångström exponent, particle depolarization) and water vapor mixing ratios, alongside with fluorescence backscatter profiles, were provided from near-ground up to 5-7 km a.s.l. Lidar-inversion algorithms were used to retrieve the aerosol microphysical properties (effective radius, single scattering albedo, and complex refractive index). The aerosol chemical composition was retrieved using the ISORROPIA thermodynamic model. The aerosol fluorescence measurements highlighted enhanced presence of bioaerosols in selected cases. Saharan dust particles exhibited high depolarization ratios (δ532 ~0.20–0.25) and lidar ratios (LR ~40–55 sr), while biomass burning plumes showed distinct microphysical and chemical signatures. Comparison of in situ and lidar-derived optical, microphysical and chemical properties at 2.314 m a.s.l. was found to be quite satisfactory, paving the way for a novel synergistic approach to further elucidate the aerosols’ role in cloud formation and radiative forcing. These lidar data are used to improve Machine Learning algorithms in the frame of the F-LIDAR-M project.

Funding: The research project, entitled “Real-time detection/Speciation of bio-aerosols profiling using Fluorescence LiDAR techniques and Machine Learning (F-LIDAR-M)” is implemented in the framework of H.F.R.I call “3rd Call for H.F.R.I.’s Research Projects to Support Faculty Members & Researchers” (H.F.R.I. Project Number: 25096).

 

How to cite: Papayannis, A. D., Gidarakou, M., Kafenidis, N., Veselovskii, I., Foskinis, R., Zografou, O., Gini, M. I., Granakis, K., Zieger, P., Jonsson, A., Schmale, J., Eleftheriadis, K., and Nenes, A.: Vertical profiling of aerosol optical, microphysical, and chemical properties using elastic-Raman-LIF lidars and in situ aerosol measurements during the 2024–2025 CHOPIN campaign, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14184, https://doi.org/10.5194/egusphere-egu26-14184, 2026.

EGU26-15933 | Posters on site | GI4.2

Vertical Wind Shear and Turbulence Detection Using Doppler Lidar and Radiosonde at NARO Space Center in South Korea 

Juseob Kim, Jung-Hoon Kim, Dan-Bi Lee, and Soo-Hyun Kim

 Atmospheric turbulence mainly induced by Vertical Wind Shear (VWS) can alter significantly the accurate positioning of space launching vehicles due to any possible distortions in their heading angles during their early stages of the flights. In this study, we developed the observation-based real-time detection system of the objective magnitude of atmospheric turbulence derived from the VWS near the NARO Space Center (NSC) in South Korea for ensuring successful launch missions of currently planned and future space vehicles. Here, we estimated an objective turbulence intensity, as a function of Eddy Dissipation Rate (EDR) that is converted from the VWS based on directly measured wind data from a Doppler wind lidar and intensive field experiments of radiosondes at the NSC for launching missions. First, we applied rigorous quality control (QC) of wind observation data to remove and filter out spurious wind data, which resulted in a high degree of agreement between the radiosonde and Doppler wind lidar measurements. This allowed us to calculate more reliable VWS to be converted to EDR using the lognormal mapping technique. Probability density functions (PDFs) of the VWS in different seasons and altitudes were established, and then used to construct the best-fit curves of prescribed lognormal function by minimizing the root mean square errors from the actual PDFs. Using the mean and standard deviation of these best-fit curves, the relationships between VWS and EDR were finally obtained and used to develop a real-time EDR estimation algorithm based on the observed wind data at the NSC. Newly developed real-time EDR estimation will provide a critical information to make a final Go or No-Go decision of the launching missions by rapidly detecting VWS-based EDR signals at the NSC site.

Acknowledgement: This work was funded by the Korea Meteorological Administration Research and Development Program under Grant KMI2022-00310 and the NARO Space Center Advancement Project of Korea Aerospace Administration.

How to cite: Kim, J., Kim, J.-H., Lee, D.-B., and Kim, S.-H.: Vertical Wind Shear and Turbulence Detection Using Doppler Lidar and Radiosonde at NARO Space Center in South Korea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15933, https://doi.org/10.5194/egusphere-egu26-15933, 2026.

EGU26-17151 | ECS | Posters on site | GI4.2

Insights into long-term Atmospheric Profiling with the Vaisala CL61 Ceilometer 

Viet Le, Ewan J. O’Connor, Maria Filioglou, and Ville Vakkari

The Vaisala CL61 is increasingly deployed in both research infrastructures, such as ACTRIS, and operational meteorological networks for applications including aviation and air-quality forecasting. As a new generation elastic backscatter lidar, it extends conventional ceilometer capabilities by providing depolarization ratio measurement. While this measurement is highly valuable, especially for unattended, autonomous operation, its use in network applications requires careful characterization.

We developed a methodology for identifying background signals and suitable liquid cloud layers to evaluate the long-term performance of multiple CL61 instruments across different sites. Results show some variability between instruments, with several of these early production units exhibiting a pronounced decrease in laser power over time, accompanied by increased background noise. Although internal calibration normally compensates for laser power degradation, external atmospheric calibration at the Lindenberg site revealed that this compensation becomes insufficient when laser power falls below 40%.

Termination hood measurements were used to characterize instrument noise and bias profiles. Both were found to exhibit temperature dependence and to deviate from zero in the near range, below approximately 2 km but extending up to 5 km for one instrument. A method for bias correction, along with an estimation of the associated uncertainty, is presented. In addition, an aerosol inversion approach is also introduced for retrieving the profile of aerosol particle backscatter coefficient, aerosol depolarization ratio, and their corresponding uncertainties. A case study demonstrates that bias-corrected, aerosol-inverted depolarization ratio can differ by up to 0.1 from the original instrument values, emphasizing the importance of accounting for instrumental bias and, in particular, molecular contributions at the CL61 operating wavelength of 905 nm.

Lastly, we observed signal loss in one instrument and found that it was due to optical lens fogging caused by insufficient internal heating linked to firmware behaviour. It is particularly important to identify and exclude such periods to ensure the reliability of the measurement.

How to cite: Le, V., J. O’Connor, E., Filioglou, M., and Vakkari, V.: Insights into long-term Atmospheric Profiling with the Vaisala CL61 Ceilometer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17151, https://doi.org/10.5194/egusphere-egu26-17151, 2026.

EGU26-18094 | ECS | Posters on site | GI4.2

From the Troposphere to Thermosphere: Compact Doppler Lidar units for observation networks 

Jan Froh, Josef Höffner, Alsu Mauer, Thorben Lüke-Mense, Ronald Eixmann, Frederik Ernst, Pablo Saavedra Garfias, Gerd Baumgarten, Alexander Munk, Sarah Scheuer, and Michael Strotkamp

We present the current status of our transportable, multi-purpose lidar units for investigating small- to large-scale processes in the atmosphere. An array of compact lidars with multiple fields of view will allow for measurements of temperatures, winds, aerosols and metals with high temporal and vertical resolution.

Our lidar units enable the investigation of Mie scattering (aerosols), Rayleigh scattering (air molecules), and resonance fluorescence (e.g. potassium atoms) from the troposphere (5 km) to the thermosphere (100 km). The unique frequency scanning laser and filter techniques allow multiple observations (wind, temperature, aerosols, metal density). The combination of a tunable alexandrite laser emitter and receiver enables high-resolution spectral characterization of the backscattered Doppler signals at day and night. In future, the relevance of such lidar networks will increase for improved weather prediction and long-term trends, monitoring of metal densities (meteoric and space debris impact) as well as calibration and validation of spaceborne missions.

We will present the progress of our lidar development in the IR and UV wavelength range, expanded measurement capabilities (e.g. aerosols, wind) and current results of measurements at 54°N and 69°N.

How to cite: Froh, J., Höffner, J., Mauer, A., Lüke-Mense, T., Eixmann, R., Ernst, F., Saavedra Garfias, P., Baumgarten, G., Munk, A., Scheuer, S., and Strotkamp, M.: From the Troposphere to Thermosphere: Compact Doppler Lidar units for observation networks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18094, https://doi.org/10.5194/egusphere-egu26-18094, 2026.

EGU26-18569 | ECS | Posters on site | GI4.2

Evaluating Turbulent Kinetic Energy Dissipation Parametrizations Using Doppler Lidars in the Convective Boundary Layer 

Syed Saqlain Abbas, Andreas Behrendt, and Volker Wulfmeyer

In mesoscale models, turbulent kinetic energy (TKE) dissipation is commonly parameterized as a function of bulk TKE, implicitly assuming isotropic turbulence in the convective boundary layer (CBL). In this study, we use long-term Doppler lidar observations at the Land-Atmosphere Feedback Observatory (LAFO), University of Hohenheim, Stuttgart, Germany to evaluate this assumption. Two continuously operated Doppler lidars, one in vertical staring mode and one in six-beam scanning mode, provide high-resolution wind measurements within the CBL (Späth et al., 2023). We have analyzed the statistical relationships between vertical velocity variance <w’2>, TKE dissipation (Wulfmeyer et al., 2024), and TKE (Bonin et al., 2017) under daytime convective conditions (06:00–18:00 UTC). The results reveal a nonlinear relationship between <w’2> and TKE, with dissipation scaling to (<w’2>)3/2. The TKE-based dissipation parametrization from Mellor-Yamada-Nakanishi-Niino (MYNN) shows only lower agreement (R2 = 0.50) with lidar observation, whereas the <w’2>-based dissipation shows a significantly stronger agreement (R2 = 0.80). Despite this difference, the turbulent length scales derived from TKE and <w’2> exhibits similar characteristics. These findings highlight limitations of bulk-TKE-based parameterizations and demonstrate the value of Doppler-lidar-based diagnostics for improving the turbulence representation in mesoscale models.

References:

Bonin et al., 2017, https://doi.org/10.5194/amt-10-3021-2017

Späth et al, 2023, https://doi.org/10.5194/gi-12-25-2023

Wulfmeyer et al, 2024, https://doi.org/10.5194/amt-17-1175-2024

How to cite: Abbas, S. S., Behrendt, A., and Wulfmeyer, V.: Evaluating Turbulent Kinetic Energy Dissipation Parametrizations Using Doppler Lidars in the Convective Boundary Layer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18569, https://doi.org/10.5194/egusphere-egu26-18569, 2026.

EGU26-19607 | ECS | Posters on site | GI4.2

Retrieval of 3 wavelengths aerosol properties from combined measurements of two ACTRIS lidar systems in troposphere and stratosphere 

Michael Haimerl, Nikolaos Siomos, Volker Freudenthaler, Hannes Vogelmann, and Michal Posyniak

Multi-wavelength lidar measurements are crucial for aerosol remote sensing as they can provide additional information for aerosol characterisation. For such measurements typically the fundamental of Nd:YAG lasers at 1064nm and the first and second harmonic at 532nm and 355nm are used. However, due to limitations in the dynamic range and quantum efficiency of detectors, signal detection for the near infrared is challenging. Accordingly, special focus lies on the contribution of our new ACTRIS CARS (Centre for Aerosol Remote Sensing) reference lidar module for 1064nm equipped with novel APD recorder setups providing high signal quality at 1064nm compared to what was possible so far. (Haimerl, 2025)  

For the EGU conference 2026 we will present intensive aerosol properties retrieved for 3 wavelengths from combined measurements in troposphere and up to lower stratosphere of the portable reference lidar system POLIS-9 of ACTRIS CARS at LMU and of the quality assured ACTRIS lidar system TONI.

The measurements were conducted in the context of an intercomparison campaign at the KIT IMK-IFU* institute in Garmisch-Partenkirchen between 01.10.2025 and 13.11.2025. The POLIS-9 reference lidar system is a combination of two portable lidar modules POLIS-6 and POLIS-1064. POLIS-6 has co- and cross-polar channels for 355nm and 532nm and vibrational Raman channels respectively. The POLIS-1064 upgrade offers 1064nm co- and cross-polar channels and a rotational Raman channel. TONI at KIT IMK-IFU is equipped with co- and cross-polar channels and vibrational Raman channels at 355nm and 532nm and a total elastic channel at 1064nm. For additional observational capabilities in the stratosphere also a lidar from KIT IMK-IFU located on nearby Zugspitze Mountain with one 532 total channel was utilized. (Haimerl, 2026) 

Aerosol products were retrieved for different aerosol cases, like smoke layers on several days during the campaign, a Saharan Dust layer on 13.11.2025 up to 4km and clean atmosphere condition on 07.11.2025. Moreover, we also try to characterise a persistent layer between 10km and 20km in the stratosphere, potentially attributed to volcanic aerosol. (Trickl, 2024)

A detailed discussion of retrieval results will then be presented at the conference. Also, we are aiming to take close overpasses of the EarthCare satellite during our campaign into account and use our retrieval results for validating the satellite data.

 

This project receives funding from European Union’s Horizon research and innovation programme under grant agreement No. 871115. ACTRIS-D is funded by German Federal Ministry for Education and Research (BMBF) under grant agreements 01LK2001A-K & 01LK2002A-G.

 

Haimerl, M. (2025) POLIS1064 – A polarization Raman lidar with state-of-the-art recorders for minimizing analogue signal distortions, Proc. European lidar conference Warsow 2025.

Haimerl, M. (2026) Retrieval of tropospheric and stratospheric aerosol properties at 3 wavelengths from combined measurements of two ACTRIS lidar systems, Proc. ACTRIS Science Conference Oslo, 2026.

Trickl, T. et. al (2024) Measurement report: Violent biomass burning and volcanic eruptions – a new period of elevated stratospheric aerosol over central Europe (2017 to 2023) in a long series of observations, Atmos. Chem. Phys., 24.

(*IMK-IFU: Institute of Meteorology and Climate Research, Atmospheric Environmental Research Department)

How to cite: Haimerl, M., Siomos, N., Freudenthaler, V., Vogelmann, H., and Posyniak, M.: Retrieval of 3 wavelengths aerosol properties from combined measurements of two ACTRIS lidar systems in troposphere and stratosphere, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19607, https://doi.org/10.5194/egusphere-egu26-19607, 2026.

EGU26-1257 | ECS | Posters on site | GI4.3

An Automated Morphometric Approach for Global Lentic and Lotic Classification of Inland Waters  

Ankit Sharma, Mukund Narayanan, and Idhayachandhiran Ilampooranan

The distinction of lentic (still) and lotic (flowing) inland waters is fundamental for understanding ecosystem functions, hydrodynamic behavior, nutrient cycling, and biogeochemical exchanges across terrestrial and aquatic interfaces. These systems influence carbon storage, sediment balance, biodiversity support, water residence time, and regional climate regulation, making accurate separation essential for large-scale hydrological assessments. However, existing classification approaches often depend on site-specific information, manual interpretation, or large training datasets, and commonly struggle to classify inland waters smaller than 3 hectares due to resolution limitations and insufficient annotated samples. This work presents an Automated Data Efficient Morphometric Approach (ADEMA) for classifying inland waters down to 0.09 ha (single LANDSAT pixel) using multi-dimensional morphometric interpretations derived using the Global Surface Maximum Extent (GSMW) dataset. The approach was trained and validated using 17,391 expert-labeled samples from 66 geographically diverse locations across multiple climate zones, varied topographies, and hydrological regimes. Further, ADEMA was benchmarked against optimized machine learning, deep learning, and global classification products. Results showed that across all size classes (small: <10 ha, medium:10-1,000 ha, and large: >1,000 ha), ADEMA provided comparable F1 scores (94%) to machine and deep learning models with minimal omission (2%), demonstrating its ability to achieve reliable classification with significantly lower computational and data requirements. A multi-decadal evaluation from 1991 to 2021 showed stable accuracy, highlighting temporal ADEMA’s robustness (F1 score = 92%). When compared to global classification products, ADEMA achieved substantially higher accuracy (average F1 score: 97% vs. 62%), especially for small and medium inland waters that are often underrepresented in global datasets. The method offers a data-efficient and automated solution suitable for regional to global hydrography. However, the framework excludes inland waters >10,000 ha to maintain computational feasibility, limiting coverage of large systems. Single-pixel detections (~0.09 ha) are less reliable due to noise, vegetation, and GSMW uncertainty, with accuracy stabilizing above ~0.5 ha. With further advancements, ADEMA could improve global open-water inventories, guide conservation strategies, and strengthen our understanding of how small inland waters collectively shape hydrology and ecosystem resilience across different environments.

How to cite: Sharma, A., Narayanan, M., and Ilampooranan, I.: An Automated Morphometric Approach for Global Lentic and Lotic Classification of Inland Waters , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1257, https://doi.org/10.5194/egusphere-egu26-1257, 2026.

EGU26-3118 | ECS | Orals | GI4.3

Assessment of chemical contamination of condensed water from Atmospheric Water Harvesting 

Thomas Merlet, Amira Doggaz, Yan Ulanowski, Stéphane Laporte, Mohamed Ali Abid, and Bérengère Lebental

As access to drinking water is a major public health issue worldwide, many technologies have emerged for water harvesting from alternative sources. Among these, active atmospheric water harvesting technologies, known as atmospheric water generators (AWGs), are attracting growing interest as a decentralised water production system. However, the water quality they produce is known to be influenced by the ambient air pollution, but scientific data on air-to-water transfer is limited, stressing the need for assessment tools to support monitoring and management strategies. This difficulty is exacerbated by the complexity of atmospheric chemistry and the large number of compounds present in the air, which far exceeds the number of compounds regulated in drinking water. To address this challenge, we present the first systematic methodology for risk assessment of air-to-AWG water transfer and apply it to the Greater Paris area. First a bibliographic inventory of the compounds found in the air in the region of interest and of their maximum reported concentration was created. For each compound, empirical (when available) or theoretical air-to-water transfer models were applied to determine the upper concentration expected in AWG water. The risk level of each compound was determined based on the ratio between this concentration and experimental or extrapolated guideline values for ingestion toxicity. In the Greater Paris area, while as many as 193 air pollutants were inventoried with quantified ground-level atmospheric concentrations over the last 15 years, only about half of them presented a risk of being present in AWG water above the set thresholds. Of these, around 20 - a much more manageable number of species to monitor - may reach concentration levels two orders of magnitude or more above the threshold values and may require priority consideration. These include ammonium, Polycyclic Aromatic Hydrocarbons -PAHs- (e.g., phenanthrene), pesticides (e.g., prosulfocarb), organic acids (e.g., acetate), phenols (e.g., benzenediol), and aldehydes (e.g., acrolein). The presence of some of these species linked to vehicle emissions was studied experimentally in the water of an AWG exposed to varying levels of diesel emissions through integrated water and air quality monitoring, both in-situ and in Sense-City climatic chamber (https://sense-city.ifsttar.fr/). A large number of species were discovered for the first time in AWG water, notably numerous PAHs and acrylamide, while several were observed to exceed EU regulatory thresholds (pH, ammonium, nitrite, Cu, Al, Mn, Pb, Ni, benzo(a)pyrene, benzene and acrylamide), some of them for the first time (Cu, acrylamide). The composition of raw AWG water was found to be directly correlated with exhaust levels through NOx and TVOC concentrations with turbidity, total organic content, nitrite, BTEX, several metals and most PAHs. Acrylamide concentration also featured correlation with the exhaust pollution, a surprising, as of yet unreported, finding in air or water that thus needs to be extensively confirmed. Overall, the study confirms the strong influence of air pollution on AWG water but its viability despite extreme pollution conditions.

How to cite: Merlet, T., Doggaz, A., Ulanowski, Y., Laporte, S., Abid, M. A., and Lebental, B.: Assessment of chemical contamination of condensed water from Atmospheric Water Harvesting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3118, https://doi.org/10.5194/egusphere-egu26-3118, 2026.

EGU26-7210 | ECS | Posters on site | GI4.3

Monitoring of the saline wedge in the rivers of the Ferrara province (Emilia Romagna region,Italy). 

Francesca Fongo and Enzo Rizzo

Saltwater intrusion threatens coastal ecosystems and water resources globally, intensified by
climate change. Rising sea levels and reduced river flows disrupt the water balance in estuarine
zones, allowing seawater to penetrate upstream into rivers and coastal aquifers. Studies predict a
9.1% global average increase in saltwater intrusion under high emissions scenarios, with extreme
events becoming up to 25 times more frequent [2]. The Po River Delta exemplifies this
vulnerability. The Ferrara area, characterized by minimal slopes and elevations mostly below sea
level, is particularly exposed. Projections indicate the Po di Goro estuary could experience up to
63% annual increase in saltwater intrusion, reaching 120% in summer [6]. The 2022 drought
demonstrated system fragility, with saltwater compromising irrigation and domestic water
supplies. Groundwater aquifers face additional stress from excessive extraction and reduced
natural recharge [1], affecting drinking water quality, agriculture, natural habitats, and soil
integrity. Traditional monitoring relies on point measurements of electrical conductivity using
boat-mounted probes, providing inadequate spatial and temporal resolution. Geophysical
methods—particularly electrical resistivity tomography (ERT) and electromagnetic (FDEM)
surveys—offer rapid, high-resolution alternatives. Previous research demonstrated the
effectiveness of combined ERT-FDEM approaches in the Po di Goro for monitoring saltwater
wedge advancement [4]. Integration of multiple geophysical techniques enables multi-scale
characterization [3].
This PhD project develops an integrated monitoring and predictive modeling system for saltwater
wedge intrusion in Ferrara, combining advanced geophysical methods with machine learning.
Building on long-term FDEM monitoring (2022-2025) in the Po di Goro, the project extends to
other Ferrara rivers and incorporates additional methods (ERT, GPR).
Expected outcomes include: (1) precise mapping of saltwater wedge extent, depth, and temporal
evolution; (2) machine learning-based predictive tools to forecast intrusion evolution; (3) decision-
support tools for sustainable water resource management, agriculture, and territorial planning,
with methodologies transferable to other estuaries globally.


The project addresses a critical gap: the absence of systematic monitoring systems and reliable
predictive tools. Increasing salinization frequency underscores the urgency for robust predictive
capabilities enabling preventive interventions. The project responds to the 2022 Po River basin
water crisis, offering practical solutions through informed policy on coastal defense, flood
mitigation, subsidence reduction, and intrusion control [5].
References
[1] Crestani, E. (2022). Large-Scale Physical Modeling of Salt-Water Intrusion. Water, 14(8), 1183.
[2] Lee, J., et al. (2025). Global increases of salt intrusion in estuaries. Nature Communications, 16,
3444.
[3] Mansourian, D., et al. (2022). Geophysical surveys for saltwater intrusion assessment. Journal
of the Earth and Space Physics, 48(3), 331–341.
[4] Rizzo, E., et al. (2023). DC and FDEM salt wedge monitoring of the Po di Goro river. EGU23-
5297.
[5] Simeoni, U. (2009). A review of the Delta Po evolution. Geomorphology, 107(1–2), 64–71.
[6] Verri, G., et al. (2024). Salt-wedge estuary's response to rising sea level. Frontiers in Climate, 6,
1408038.

How to cite: Fongo, F. and Rizzo, E.: Monitoring of the saline wedge in the rivers of the Ferrara province (Emilia Romagna region,Italy)., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7210, https://doi.org/10.5194/egusphere-egu26-7210, 2026.

EGU26-10394 | Orals | GI4.3

Characterization of Offshore Freshened Groundwater systems on the Ross sea shelf 

Francesco Chidichimo, Ariel Tremayne Thomas, Michele De Biase, Salvatore Straface, and Aaron Micallef

Offshore Freshened Groundwater (OFG) is increasingly recognized as an important component of continental shelf hydrogeology, yet its physical structure, geochemical evolution, and preservation mechanisms remain poorly documented in polar settings. This study characterizes OFG systems on the Ross Sea shelf using borehole porewater data from IODP (Integrated Ocean Drilling Program) Sites U1522 and U1524, with the aim of resolving their vertical structure, origin, and diagenetic state.

Depth-resolved porewater samples were analyzed for chloride, stable water isotopes (δ¹⁸O, δ²H), major cations and anions, and redox-sensitive species. Lithological information was used to assess stratigraphic controls on fluid distribution. A groundwater transport model was applied to evaluate the relative roles of diffusive and advective processes in shaping present-day porewater profiles.

Both sites host vertically stratified OFG systems comprising a saline, marine-influenced upper unit, an intermediate transition zone, and a deeper freshened interval preserved beneath finer-grained sediments. Downcore decreases in chloride and progressive depletion of δ¹⁸O and δ²H indicate dilution by a non-marine water source, while elevated Br/Cl ratios and smooth concentration gradients support long residence times and limited modern exchange. Redox profiles show sulfate depletion, ammonium enrichment, and methane production at depth, indicating active diagenetic alteration of the fluids. The transport model demonstrates that diffusion is the dominant control on present-day tracer distributions, with only minor or negligible vertical flow patterns.

The Ross Sea OFG systems at Sites U1522 and U1524 are therefore laterally extensive, vertically stratified, and geochemically evolved bodies, preserved through stratigraphic confinement and diffusion-dominated transport. Their characteristics reflect long-term isolation and water-rock interaction rather than active recharge phenomena, highlighting OFG as a stable subsurface reservoir and an archive of past hydrogeological conditions on polar continental shelves.

How to cite: Chidichimo, F., Thomas, A. T., De Biase, M., Straface, S., and Micallef, A.: Characterization of Offshore Freshened Groundwater systems on the Ross sea shelf, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10394, https://doi.org/10.5194/egusphere-egu26-10394, 2026.

EGU26-11204 | ECS | Orals | GI4.3

Preliminary results of a cost-effective optical imaging and deep learning system for algal bloom monitoring in Lake Lugano  

alessandro centazzo, daniele strigaro, claudio primerano, massimiliano cannata, and camilla capelli

Algal blooms represent a significant challenge for the sustainable management of freshwater habitats, strongly affecting water quality, biodiversity, ecosystem functioning, and human activities. Their occurrence is often driven by complex interactions between natural processes and anthropogenic pressures [1–3]. Consequently, there is a growing demand for monitoring strategies capable of capturing the spatial and temporal variability of algal dynamics while supporting a holistic assessment of water habitat health. Traditional monitoring approaches typically rely on point-scale in situ measurements or satellite remote sensing products, which, although essential, are often limited by spatial resolution, revisit frequency, operational costs, or deployment constraints [4]. In this context, low-cost, image-based sensing systems represent a promising complementary solution, enabling continuous and visually explicit observations at local to regional scales. 

This contribution presents preliminary results from an in situ monitoring system based on cost-effective optical imaging cameras combined with deep learning-based image analysis. The proposed approach is developed within the framework of the WINCA4TI (Water Interactions with Nature, Climate and Agriculture for Ticino) Interreg project, which aims to foster cross-border innovation in environmental monitoring through low-cost sensing technologies and data-driven methods. The system is designed to complement high-end in situ instrumentation and satellite observations by providing flexible, scalable, and cost-effective monitoring capabilities, with a specific focus on the automatic characterization of algal bloom phenomena to support near-real-time detection and decision making. 

The monitoring system relies on compact cameras and optical sensors operating in the visible and near-infrared spectral ranges, deployed on fixed platforms suitable for long-term observations and on-site (edge) processing. Image data are initially combined with in situ measurements to build a reliable reference dataset, which is subsequently exploited to enable image-only monitoring. The computational workflow integrates image preprocessing, including illumination normalization and water surface masking, with deep learning–based image segmentation to derive spatial and temporal indicators of algal presence, surface coverage, and bloom dynamics. 

Preliminary results demonstrate the capability of the proposed approach to capture fine-scale spatial and temporal patterns of algal blooms, bridging the gap between localized field measurements and large-scale remote sensing products. The findings suggest that low-cost image-based monitoring systems can enhance the responsiveness and resilience of water management strategies, particularly where traditional monitoring is constrained by cost, logistics, or spatial coverage. 

 

  • Strigaro D., Capelli C. (2024). An open early-warning system prototype for managing and studying algal blooms in Lake Lugano. https://doi.org/10.5194/isprs-archives-XLVIII-4-W12-2024-143-2024 
  • Bosse K. R., Fahnenstiel G. L., Buelo C. D., Pawlowski M. B., Scofield A. E., Hinchey E. K., & Sayers M. J. (2024). Are harmful algal blooms increasing in the Great Lakes? https://doi.org/10.3390/w16141944 
  • Zeng K., Gokul E. A., Gu H., Hoteit I., Huang Y., & Zhan P. (2024). Spatiotemporal expansion of algal blooms in coastal China seas.  https://doi.org/10.1021/acs.est.4c01877 
  • Ogashawara I. (2019). Advances and limitations of using satellites to monitor cyanobacterial harmful algal blooms. https://doi.org/10.1590/S2179-975X0619 

How to cite: centazzo, A., strigaro, D., primerano, C., cannata, M., and capelli, C.: Preliminary results of a cost-effective optical imaging and deep learning system for algal bloom monitoring in Lake Lugano , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11204, https://doi.org/10.5194/egusphere-egu26-11204, 2026.

EGU26-13495 | Posters on site | GI4.3

Advances in supraglacial lake detection and characterization on the Nansen Ice Shelf from active microwave and visible light satellite remote sensing 

Francesco De Biasio, Stefano Vignudelli, Stefano Zecchetto, Matteo Zucchetta, Emiliana Valentini, Marco Salvadore, and Roberto Salzano

The evolution of cryospheric components (snow cover, ice, and meltwater) plays a fundamental role in regulating energy exchanges between the atmosphere and ice shelves and represents a key indicator of climate change impacts in remote polar regions. Within the framework of the HOLISTIC (Holistic Overview of the supraglacial Lake–Ice–Snow Timing and Climate causality) project, funded by the Italian National Antarctic Research Program, we present an advanced multi-sensor assessment of supraglacial lake (SGL) dynamics over the Nansen Ice Shelf (Victoria Land, Antarctica).

We adopted a synergistic remote sensing approach, aimed at integrating active microwave observations from satellite SAR and radar altimetry missions with optical imagery. This multi-frequency and multi-platform strategy investigates the possibility of detection, mapping and temporal monitoring of SGL position and extent and spatial distribution under all-weather conditions and across different spatial and temporal scales. HH-polarized SAR data proved effective in identifying surface meltwater signatures and characterizing seasonal lake evolution, despite polarization limitations, while optical data provided complementary constraints on lake morphology and surface hydrology during cloud-free periods. The seasonal melt and refreezing processes of SGL units were further investigated by leveraging the combined revisit time of operational sensors such as Sentinel-2 and Landsat, together with dedicated tasking missions like PRISMA, providing a more comprehensive understanding of lake dynamics over time.

A dedicated processing chain for Sentinel-3 altimetry L1A individual echoes was implemented using the PISA algorithm (Abileah and Vignudelli, 2021, https://doi.org/10.1016/j.rse.2021.112580). This allowed the retrieval of localized elevation anomalies associated with bright targets, mountainous targets and supraglacial water bodies, and the characterization of surface roughness changes presumably linked to melt and drainage processes, as well as to changes in snow density and surface slope.

The combined analysis highlights the strong coupling between snowpack evolution, surface energy feedback, and the formation and drainage of SGLs, providing new insights into ice-shelf surface hydrology and its seasonal to interannual variability. The results represent a step forward in quantifying SGL properties using active microwave and passive/active optical techniques and offer a valuable testbed for existing and future altimetry missions, such as NASA's ICESat-2 and ESA’s CRISTAL missions, aimed at directly retrieving snow depth. The capabilities of high-resolution satellite-born SAR sensors are also expected to benefit from this study, in detecting and monitoring snowpack changes, particularly those resulting from surface snow melt and the formation of supraglacial lakes. Supraglacial lakes emerge as particularly suitable targets for assessing visible light as well as Ka-, Ku- and C-band scattering contributions and for advancing the understanding of snow–ice–water interactions in polar environments.

How to cite: De Biasio, F., Vignudelli, S., Zecchetto, S., Zucchetta, M., Valentini, E., Salvadore, M., and Salzano, R.: Advances in supraglacial lake detection and characterization on the Nansen Ice Shelf from active microwave and visible light satellite remote sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13495, https://doi.org/10.5194/egusphere-egu26-13495, 2026.

EGU26-14117 | ECS | Orals | GI4.3

Coastal and Land Use Variations of Burullus Lake, Egypt Using Remote Sensing  

Elsayed Abdelsadek, Salwa Elbeih, and Abdelazim Negm

Monitoring lakes is traditionally expensive, but satellite technology offers a more affordable solution. Human activities are currently damaging water bodies worldwide, including Egypt's coastal lakes. This study focuses on Burullus Lake, Egypt’s second-largest lake in the northern Mediterranean. Researchers used Remote Sensing and Geographic Information Systems (GIS) to track changes in the coastline and land use. The authors analyzed Landsat images from 1984 to 2019 and compared 2019 Landsat data with Sentinel-2A imagery. They also performed field visits to confirm their findings. Using a supervised classification method, they identified eight categories, including seawater, urban areas, and fish farms.

The results show significant changes between 1984 and 2019: the lake’s open water decreased by 16%, and floating plants dropped by 52%. Conversely, agricultural land expanded by 648 km^2, and fish farms grew by 290 km^2. These updated maps help officials identify where human activity is most harmful. This data is essential for restoring the lake and meeting Sustainable Development Goals (SDGs).

Keywords: Remote Sensing & GIS, Environmental Monitoring, Land Use/Land Cover (LULC), Change Detection, Burullus Lake, Egypt,

How to cite: Abdelsadek, E., Elbeih, S., and Negm, A.: Coastal and Land Use Variations of Burullus Lake, Egypt Using Remote Sensing , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14117, https://doi.org/10.5194/egusphere-egu26-14117, 2026.

EGU26-14855 | Posters on site | GI4.3

Benchmarking UAV multispectral sensors and machine learning for water quality estimation 

Caio Mello, Daniel Salim, Bernardo Souza, Gabriel Pereira, and Camila Amorim

The sustainable management of water resources in anthropogenic contexts requires a holistic transition from mere monitoring to comprehensive assessments of water habitats. Urban reservoirs are particularly vulnerable ecosystems, where pressures such as agricultural runoff and untreated sewage discharge drive eutrophication, compromising water quality. Traditional monitoring methods often lack the spatiotemporal resolution required to capture the complex dynamics of these environments. To address this gap, this study evaluates the efficacy of close-range remote sensing combined with Machine Learning (ML) and Explainable Artificial Intelligence (XAI) for estimating optically active water quality parameters (turbidity, chlorophyll-a, and phycocyanin). The research was conducted at the Ibirité Reservoir (Minas Gerais, Brazil), a highly eutrophic urban system serving as a petrochemical industry water supply. Ten monthly field campaigns (August 2024 to May 2025) were conducted, covering both dry and wet seasons, to capture seasonal variability. Data acquisition employed Unmanned Aerial Vehicles (UAVs) equipped with two distinct multispectral sensors: the DJI Phantom 4 Multispectral (P4M – 5 bands) and the MicaSense RedEdge Dual-P (MSR – 10 bands). This setup allowed for a comparative analysis of spectral resolution impacts on model performance. The methodology tested three ML algorithms: Random Forest, CatBoost, and XGBoost. To ensure physical consistency, SHAP (SHapley Additive exPlanations) values were used to interpret the models. This ML-XAI approach assessed: (1) the comparative performance of each sensor and algorithm; and (2) the robustness of the models by identifying the most influential spectral bands for each parameter. Results indicate that ensemble learning algorithms, specifically Random Forest and CatBoost, consistently outperformed others across datasets. The MSR sensor achieved the highest overall accuracy, particularly for Phycocyanin estimation using Random Forest (R² = 0.93), compared to the P4M's best result for the same parameter (R² = 0.90). Explainable AI analysis revealed the physical drivers behind this performance: for Phycocyanin, the MicaSense models relied heavily on the specific 717 nm and 705 nm (RedEdge) bands. This explains the superior performance, as these narrow bands better resolve the specific spectral features of cyanobacteria compared to the single RedEdge band available on the DJI sensor. Conversely, for Chlorophyll-a, the NIR (842 nm) and Red (650 nm) bands were the dominant predictors. Since both sensors possess these bands, the performance gap was narrower (R² = 0.79 for MSR vs. 0.77 for P4M), validating the cost-effectiveness of the 5-band sensor for general pigment monitoring. However, for Turbidity, the additional spectral resolution of the MSR (specifically the 717 nm band) proved decisive, raising accuracy to R² = 0.84 compared to 0.78 for the P4M. Findings demonstrate that integrating high-resolution multispectral sensing with interpretable ensemble learning offers a scalable and physically consistent tool for monitoring water habitat health, supporting data-driven decision-making in complex urban environments.

How to cite: Mello, C., Salim, D., Souza, B., Pereira, G., and Amorim, C.: Benchmarking UAV multispectral sensors and machine learning for water quality estimation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14855, https://doi.org/10.5194/egusphere-egu26-14855, 2026.

EGU26-18033 | ECS | Orals | GI4.3

MaD-OPS: Monitoring & Detection of Organic Pollution from Sewage: Implementation of an agile sensing network for informing river health 

Connie Tulloch, Rosie Perrett, Matthew Coombs, Izaak Stanton, John Attridge, Robin Thorn, Lyndon Smith, and Darren Reynolds

Rivers are under pressure from many different sources, including farming and rural land use, wastewater treatment, towns and transport. In England, very few rivers achieve good ecological status, and none achieve good chemical status. This comes after many years of exploiting our freshwater systems. In 2024 there were more than 450,000 combined sewer overflow discharges in England, totalling over 3.5 million hours of spills. This sewage has direct implications on ecological and human health, increasing the environmental contaminant load in rivers. In response, Section 82 of the Continuous Water Quality Monitoring Programme mandates continuous monitoring of freshwater systems, with scope for future expansion of monitored parameters.  

Current water quality monitoring relies heavily on infrequent spot sampling, often missing key impact events, with limited spatiotemporal context. The MaD-OPS project has developed a novel sensing network for continuous monitoring of biological, chemical, and physical water quality parameters. A key focus is to demonstrate the value of a new fluorescence-based optical sensor for detecting organic pollution and bacterial contamination within a demonstrator catchment, with the potential to reveal underlying biogeochemical cycling processes. 

To isolate different pollution sources, sensor nodes have been deployed at multiple points along a river. Alongside continuous sensor data, regular spot sampling is being carried out for faecal indicator organisms, BOD₅, nutrient analysis, and microbial community profiling to provide robust ground-truthing.  

The project aims to develop a user-friendly dynamic Water Quality Index (WQI) that integrates high-frequency sensor data with machine learning, for real time assessment of river health that can be used by citizen scientists, community groups, and regulators alike. Using a novel dynamic baseline approach, the WQI will assess each sensor node relative to the least impacted section of the river at any given time.  

Preliminary results demonstrate that continuous monitoring captures point source pollution and hydrological events that are not detected through spot sampling alone. Comparison between the dynamic headwater baseline and downstream sensor nodes highlights the direct impact of point source events on river health.  

We present progress in deploying the sensing network, early insights into river health derived from high-frequency data, and how these findings are informing the development of the WQI framework. 

 

How to cite: Tulloch, C., Perrett, R., Coombs, M., Stanton, I., Attridge, J., Thorn, R., Smith, L., and Reynolds, D.: MaD-OPS: Monitoring & Detection of Organic Pollution from Sewage: Implementation of an agile sensing network for informing river health, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18033, https://doi.org/10.5194/egusphere-egu26-18033, 2026.

EGU26-18415 | ECS | Posters on site | GI4.3

Selective Fluorescence Sensing of Methylene Blue Dye Using Yeast-Based Carbon Dots: Experimental and Computational Study 

Neeraj Chauhan, Stefan Krause, Manjinder Singh, and Amrit Pal Toor

Synthetic dyes released from textile and related industries are a major source of aquatic pollution and can pose risks to ecosystem and human health. Methylene blue (MB), a widely used cationic thiazine dye in industrial dyeing and pharmaceutical applications, is of particular concern because it can persist in water and affect photosynthetic activity, aquatic biodiversity, and water quality. However, monitoring dye contamination often relies on laboratory-based analytical techniques that are costly and time-consuming, limiting rapid assessment in field conditions.

In this study, yeast powder (a low-cost and renewable bio-precursor) was converted into fluorescent carbon dots (C-dots) using a simple one-pot hydrothermal synthesis route. The as-prepared C-dots showed excitation-dependent fluorescence emission with a clear red shift from 360 to 460 nm. Structural and chemical characterisation using UV–Vis, TEM, XPS, XRD, FTIR and Raman spectroscopy confirmed quasi-spherical particles with an average size of 3–8 nm and an amorphous carbon structure enriched with oxygen-containing functional groups. The C-dots exhibited high stability across a wide range of pH and salinity (NaCl), under prolonged UV exposure and during storage.

The C-dots were then applied as a fluorescence-based sensor for rapid and selective detection of methylene blue in water. A strong decrease in fluorescence intensity was observed upon addition of MB, with a linear response in the range of 1 ppb to 1 ppm. The sensor achieved a limit of detection (LOD) of 73.9 ppb and a limit of quantification (LOQ) of 246.4 ppb, demonstrating high sensitivity. The sensing mechanism was attributed to fluorescence quenching dominated by FRET, supported by experimental spectroscopy and computational investigations. Theoretical analysis further indicated that π–π stacking and hydrogen bonding interactions between MB molecules and the C-dot surface contribute to strong binding and enhanced selectivity.

Finally, the developed sensor was successfully applied to real water samples, showing satisfactory recoveries between 96% and 116%. Overall, this work demonstrates a green, cost-effective and highly sensitive fluorescent nanosensor for MB monitoring, offering strong potential for real-time water quality assessment and pollution control in freshwater and wastewater systems.

How to cite: Chauhan, N., Krause, S., Singh, M., and Toor, A. P.: Selective Fluorescence Sensing of Methylene Blue Dye Using Yeast-Based Carbon Dots: Experimental and Computational Study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18415, https://doi.org/10.5194/egusphere-egu26-18415, 2026.

EGU26-18591 | ECS | Orals | GI4.3

Monitoring Contaminants of Emerging Concern and eDNA off the Coast of Ireland Using Autonomous Surface Vehicles: A Spatiotemporal Study 

Nicolette Sale, Fiona Regan, Anne Parle-McDermott, Michelle Wosinski, Gerard Dooly, Luke Griffin, Dinesh Babu Duraibabu, Paulo Prodöhl, and M. Isabel Cadena-Aizaga

Contaminants of emerging concern (CECs), including pharmaceuticals, pesticides, and PFAS, have attracted increased attention due to their potential to affect the environment and human health. At the same time, environmental DNA (eDNA) can detect and monitor biological communities and can complement chemical monitoring to give a more comprehensive picture of ecosystem status. The simultaneous sampling of CECs and eDNA presents significant technical and logistical challenges and requires very sensitive techniques. Autonomous surface vehicles (ASVs) offer a flexible platform for monitoring coastal water systems, particularly when repeated or prolonged sampling is required. Their use is increasingly relevant for supporting emerging biological and chemical monitoring techniques. Despite its potential, few studies investigate seawater ecosystems using this combined approach. 

 

This work involves innovative monitoring of Irish coastal waters using an interdisciplinary approach that integrates expertise in engineering, chemistry, and biology. Research involving an ASV capable of reliable dynamic positioning during extended sampling operations will be shown alongside sensitive analytical techniques for investigating CECs and eDNA in seawater matrices. Results will show strategies to address a key challenge for ASV-based eDNA sampling of maintaining precise station for adequate periods while water is actively pumped through our filtration systems. Study observations include methods for sample handling to overcome the challenge of low target analyte concentration degradation, and contamination.

How to cite: Sale, N., Regan, F., Parle-McDermott, A., Wosinski, M., Dooly, G., Griffin, L., Duraibabu, D. B., Prodöhl, P., and Cadena-Aizaga, M. I.: Monitoring Contaminants of Emerging Concern and eDNA off the Coast of Ireland Using Autonomous Surface Vehicles: A Spatiotemporal Study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18591, https://doi.org/10.5194/egusphere-egu26-18591, 2026.

EGU26-18973 | Posters on site | GI4.3

Quantifying early seagrass growth with UAV imagery 

Matteo Albéri, Mohamed Abdelkader, Cinzia Cozzula, Federico Cunsolo, Nedime Irem Elek, Engin Can Esen, Ghulam Hasnain, Fabio Mantovani, Michele Mistri, Cristina Munari, Maria Grazia Paletta, Marco Pezzi, Kassandra Giulia Cristina Raptis, Andrea Augusto Sfriso, Adriano Sfriso, and Virginia Strati

Within the framework of proximal sensing, monitoring early-stage seagrass colonization in turbid waters presents challenges due to the spectral similarity between the dwarf eelgrass Zostera noltei and ephemeral macroalgae. A preliminary study previously demonstrated the utility of high-resolution Unmanned Aerial Vehicle (UAV) imagery for general monitoring through visual inspection (Mistri et al., 2025). However, the reliance on manual detection and known transplantation coordinates limits the scalability of the approach. In this study, we take a further step to overcome these limitations by applying pixel-based supervised classification to high-resolution orthomosaics. This allows for precise and quantitative tracking of the spatial evolution of seagrass meadows over time.

Ultra-high-resolution aerial surveys were conducted in the Caleri Lagoon (Po River Delta, Italy) using a DJI Air 2S UAV flown at an altitude of 7 meters, achieving a theoretical ground sampling distance of 0.2 cm/pixel. The collected imagery was processed into georeferenced orthomosaics and analyzed using a supervised Maximum Likelihood Classification algorithm based on Bayes’ theorem. To isolate the spectral signal of the target seagrass, the probabilistic framework incorporated 40 regions of interest for each of five classes: seagrass, green algae, red algae, shadow, and background. To reduce high-frequency 'salt-and-pepper' noise, a post-classification Sieve filter (20×20 pixel window) was applied, refining patch segmentation based on neighborhood mode.

Multitemporal analysis revealed a distinct non-linear expansion trajectory within the 0.5-hectare study area. Starting from a planted footprint of just 2.5 m² (~0.05% of the study area) in August 2023, the seagrass colonies expanded to 60 m² (1.2%) by June 2024, reaching approximately 716 m² (14%) by October 2025.

These results demonstrate that combining low-altitude UAV photogrammetry with probabilistic classification offers a highly repeatable and scalable framework for quantifying restoration dynamics. This methodology effectively overcomes the limitations of manual monitoring, enabling the detection of the subtle, non-linear growth patterns typical of early-stage colonization.

How to cite: Albéri, M., Abdelkader, M., Cozzula, C., Cunsolo, F., Elek, N. I., Esen, E. C., Hasnain, G., Mantovani, F., Mistri, M., Munari, C., Paletta, M. G., Pezzi, M., Raptis, K. G. C., Sfriso, A. A., Sfriso, A., and Strati, V.: Quantifying early seagrass growth with UAV imagery, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18973, https://doi.org/10.5194/egusphere-egu26-18973, 2026.

Machine learning (ML) models have become essential tools for monitoring water system dynamics, enabling accurate prediction of water levels, discharge patterns, and responses to meteorological forcing. However, their operational deployment remains constrained by limited interpretability and the challenge of translating numerical outputs into actionable insight, particularly when assessing system anomalies, regime shifts, and potential impacts on aquatic and riparian habitats.

This study introduces a novel framework that integrates large language models (LLMs) as a semantic interpretation layer within ML-based hydrological monitoring systems. Building on established time-series ML architectures for water level prediction, model outputs are coupled with statistical anomaly detection techniques to identify atypical hydrological behaviour, threshold exceedances, and periods of elevated system stress relevant to near-real-time monitoring. These quantitative signals, together with meteorological drivers and system metadata, are subsequently processed by an LLM to generate structured, contextual natural-language explanations.

The proposed framework is demonstrated using historical water monitoring datasets, with particular emphasis on extreme events and hydrological anomalies. When such events are detected, the LLM synthesizes information across multiple data streams to articulate observed patterns, plausible hydro-meteorological drivers, and potential implications for water system functioning and associated habitats. Rather than replacing process-based understanding or predictive models, the LLM acts as an intelligent synthesis component that contextualizes ML outputs and supports their interpretation.

Results indicate that LLM-enhanced monitoring outputs can substantially improve transparency, interpretability, and communicability compared to conventional numerical monitoring approaches, thereby facilitating improved situational awareness and decision support during critical periods. By embedding natural-language reasoning within data-driven monitoring workflows, this work establishes a pathway toward interpretable, stakeholder-centred hydrological monitoring that aligns advanced artificial intelligence methods with practical environmental observation and management needs.

Keywords

  • Hydrological monitoring
  • Machine learning interpretability
  • Large language models
  • Water system intelligence

How to cite: slaimi, A. and Scriney, M.: Explainable Hydrological Monitoring: Large Language Models as Semantic Interpreters of Machine-Learning-Based Water System Intelligence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19125, https://doi.org/10.5194/egusphere-egu26-19125, 2026.

EGU26-19151 | ECS | Orals | GI4.3

Open-Source Fluorescence Sensing with a Turbidity Correction Model for Community-based Freshwater Monitoring 

Riccardo Cirrone, Francesco Vesprini, Amedeo Boldrini, Alessio Polvani, Xinyu Liu, Luisa Galgani, and Steven Loiselle

Monitoring and maintaining functioning freshwater habitats is increasingly challenging, despite the widespread implementation of European and international freshwater quality monitoring frameworks. With the complexities of climate change, there is a need for data with higher spatial and temporal resolution. In this context, citizen science initiatives have emerged as a valuable complement to official monitoring programs. These initiatives are particularly important in small river basins and remote rural areas, where data from environmental agencies is often sparse or unavailable. However, concerns regarding the reliability and consistency of citizen-generated data persist, highlighting the need for novel technological solutions capable of improving the quality of in situ measurements collected by volunteers.

We present a low-cost fluorometer for field measurements of phytoplankton biomass, through the measurement of chlorophyll-a, featuring a multivariate turbidity correction algorithm and automated online data upload. This open-source device aims to advance monitoring by integrating cutting-edge optical sensing with IoT connectivity and citizen science.
The sensor is integrated in a 3D-printed case and comprises an optical system with two light sources: an 820 nm LED for turbidity measurements and a 430 nm SMD LED for chlorophyll-a excitation, coupled with a long-pass optical filter. The voltage signal from the photodiode is acquired via a 16-bit analog-to-digital converter and transmitted to a microcomputer (Raspberry Pi Zero 2 W), which powers and controls the system.
Laboratory and field evaluations demonstrated that the sensor delivers accurate and reproducible measurements, achieving higher resolution and precision than measurements without turbidity correction. For ease of replication, the 3D enclosure CAD model, software, and user guidelines are openly accessible online.

How to cite: Cirrone, R., Vesprini, F., Boldrini, A., Polvani, A., Liu, X., Galgani, L., and Loiselle, S.: Open-Source Fluorescence Sensing with a Turbidity Correction Model for Community-based Freshwater Monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19151, https://doi.org/10.5194/egusphere-egu26-19151, 2026.

EGU26-19435 | ECS | Orals | GI4.3

Towards an Assessment of Atmospheric Forcing on Chlorophyll-a and Turbidity in an Oligotrophic Lake: Lake Bolsena Case Study 

Valentina Terenzi, Mariano Bresciani, Cludia Giardino, Anna Joelle Greife, Monica Pinardi, Patrizio Tratzi, Flaminia Fois, and Cristiana Bassani

Chlorophyll-a (Chl-a) is commonly used as an indicator of phytoplankton biomass and eutrophication in inland waters, as it reflects changes in primary productivity and nutrient availability. Turbidity describes the optical effect of suspended particles in the water column and, in oligotrophic lakes, is typically low but highly responsive to external factors such as wind-induced mixing and precipitation. Analyzing Chl-a and turbidity together in relation to atmospheric conditions is therefore crucial for evaluating water quality and identifying potential pressures on aquatic ecosystems.
In this study, Lake Bolsena was investigated as a representative oligotrophic system to evaluate how atmospheric conditions influence Chl-a concentration and turbidity. The analysis was conducted over the lake surface and an additional surrounding land buffer of approximately 15 km, selected to account for meteorological and atmospheric processes that are not confined to the water body itself but can indirectly affect its optical and biological properties.
Chl-a and turbidity were derived from the data set (version 2.1) of the ESA Lakes_cci project based on the processing of OLCI images for the period 2016-2022. Meteorological variables considered include wind speed at 10m, 2-m air temperature, surface pressure, boundary layer height, precipitation, and solar radiation, all derived from the ERA5 reanalysis dataset (Hersbach et al., 2020). In oligotrophic lakes, wind speed regulates water column mixing and sediment resuspension, while air temperature and solar radiation influence thermal stratification and the energy available for phytoplankton growth; precipitation contributes to suspended material modifying surface optical properties. Boundary layer height and surface pressure provide additional information on atmospheric stability and mixing conditions that modulate air–water exchanges.
Aerosol Optical Depth (AOD) retrieved using the MAIAC algorithm was also included, although it is not available directly over the lake surface but only in the surrounding area (Lyapustin et al., 2018). AOD was used as a proxy for regional aerosol loading to investigate its potential indirect effects on the lake through dry and wet deposition of particulate matter and nutrients, which may alter water transparency and, over time, phytoplankton dynamics even under oligotrophic conditions.
Correlation analysis revealed significant seasonal variability throughout the studied period. Chl-a is particularly influenced by multiple atmospheric forces in autumn, while turbidity is primarily driven by meteorological factors in summer. Both water quality parameters exhibit variable but significant dependencies in spring; on the other hand, atmospheric influence is less relevant in winter.
References
Hersbach, H., et al. (2020). The ERA5 global reanalysis. Quarterly Journal of the Royal Meteorological Society, 146, 1999–2049, https://doi.org/10.1002/qj.3803
Lyapustin, A., Wang, Y., Korkin, S., and Huang, D.: MODIS Collection 6 MAIAC algorithm, Atmos. Meas. Tech., 11, 5741–5765, https://doi.org/10.5194/amt-11-5741-2018, 2018.

How to cite: Terenzi, V., Bresciani, M., Giardino, C., Greife, A. J., Pinardi, M., Tratzi, P., Fois, F., and Bassani, C.: Towards an Assessment of Atmospheric Forcing on Chlorophyll-a and Turbidity in an Oligotrophic Lake: Lake Bolsena Case Study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19435, https://doi.org/10.5194/egusphere-egu26-19435, 2026.

EGU26-21301 | ECS | Orals | GI4.3

Advancing Water Data Ecosystems: Identifying and Optimizing Connectivity and Beyond-Connectivity Requirements with 5G/6G Technologies 

Abdelhak Kharbouch, Mehdi Monemi, Pirkko Taskinen, and Mehdi Rasti

This paper examines the connectivity and beyond-connectivity requirements essential for water data ecosystems, highlighting the critical role of advanced communication technologies, such as 5G/6G, in enabling rapid, reliable data transmission for real-time monitoring and decision-making. Optimizing communication protocols supports robust infrastructure, interoperability among diverse sources, including environmental sensors, weather data, and utility-provided information, and seamless data integration and utilization, while promoting innovation, efficiency, and sustainability in water management.

The study is structured in two main parts. First, it identifies specific connectivity and beyond-connectivity requirements, focusing on the integration of various water data sources and evaluating the efficacy of communication protocols to support dynamic data integration, including capabilities like artificial intelligence, sensing, and sustainability. This forms the foundation for subsequent analysis. Second, it analyzes and optimizes connectivity services offered by 5G/6G and beyond technologies to meet these requirements, considering factors such as energy efficiency, reliability, scalability, and integrated services like sensing, AI, and computation.

The study aims to demonstrate that addressing these requirements enhances the integration and utilization of diverse water data, facilitating access to information, development of new solutions, improved understanding of water management challenges, and innovation in water supply through enhanced prediction models and more efficient, sustainable solutions. It identifies and optimizes key performance indicators (KPIs) as well as services derived from standardization bodies, tailored to water-related use cases such as leak detection, wastewater monitoring, and resource efficiency. These include ultra-low latency for critical alerts, high reliability for infrastructure control, energy efficiency in sensor networks, scalability for IoT-dense environments, and integrated AI for dynamic data processing. Anticipated insights reveal how water data ecosystems can overcome challenges like demand-supply gaps through efficient data collection, sharing, and utilization, while addressing barriers such as limited data availability and regulatory constraints. This necessitates clear visions, effective data-sharing mechanisms, and scalable architectures to drive innovation and reduce water loss.

The proposed framework facilitates informed strategies and new opportunities for stakeholders in water utilities and related sectors. This study advances the understanding of digitalization in critical infrastructure, demonstrating how optimized connectivity can promote efficiency and sustainability in water management.

How to cite: Kharbouch, A., Monemi, M., Taskinen, P., and Rasti, M.: Advancing Water Data Ecosystems: Identifying and Optimizing Connectivity and Beyond-Connectivity Requirements with 5G/6G Technologies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21301, https://doi.org/10.5194/egusphere-egu26-21301, 2026.

EGU26-22477 | Posters on site | GI4.3

Spatial Dynamics of Mercury and Phytoplankton in Lake Maggiore: An Integrated Monitoring Approach 

Martina Austoni, Laura Fantozzi, and Giorgio Luciano

Mercury contamination in freshwater ecosystems is of major concern due to its persistence, toxicity, and bioaccumulation potential.  This preliminary study investigates mercury dynamics in Lake Maggiore by integrating surface water mercury analyses with high-resolution assessments of phytoplankton structure and chlorophyll concentrations along the water column and surface water. Monitoring activities were conducted using FluoroProbe probe (BBE Moldaenke GmbH) to characterize algal groups with particular focus on the horizontal spatial distribution of both chlorophyll and mercury in proximity to tributaries and lake outlets. Surface water samples were analyzed for mercury concentrations using a Lumex RA‑915+ portable atomic absorption spectrometer, equipped with the dedicated attachment for dissolved and total mercury determination in water, while FluoroProbe profiles were used to quantify algal group composition and chlorophyll distribution. Results reveal marked spatial heterogeneity in mercury concentrations, closely associated with tributary zones and changes in chlorophyll patterns, suggesting coupling between hydrological inputs, phytoplankton dynamics, and mercury behavior. This integrated monitoring approach improves understanding of mercury–ecosystem interactions in large lake systems and supports the development of effective monitoring and management strategies for freshwater environments.

How to cite: Austoni, M., Fantozzi, L., and Luciano, G.: Spatial Dynamics of Mercury and Phytoplankton in Lake Maggiore: An Integrated Monitoring Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22477, https://doi.org/10.5194/egusphere-egu26-22477, 2026.

EGU26-1296 | Posters on site | GI4.4

Seismo-Volcanic Crises Across the Red Sea and East African Rifts: The Critical Role of New Projects and International Collaborations in Data-Poor Regions 

Elias Lewi, Tesfaye Temtime, Juliet Biggs, Atalay Ayele, Tim Wright, Carolina Pagli, Derek Keir, and Susan Loughlin,

In recent years, segments of the Red Sea Rift System (Erta Ale, Hayli Gubbie, areas around Atsbi) and the East African Rift System (Fentale) have experienced intensified seismo-volcanic activity, highlighting the urgent need for enhanced monitoring across Ethiopia’s tectonically active regions. Between July and August 2025, Erta Ale underwent a significant magmatic and diking episode propagating southward toward Afder, followed by renewed activity culminating in the November 2025 eruption at Hayli Gubbie, 11.6km southeast of the Erta Ale lava lake. In the region around Atsbi, seismic sequences in October 2025 appear primarily seismo-tectonic, though potential deeper magmatic involvement remains uncertain. On the other hand, the Fentale region of the East African Rift System exhibited sustained seismicity and deformation from September 2024 to March 2025, affecting nearby communities and infrastructure. Despite the scientific significance of these events, Ethiopia faces challenges in maintaining and expanding geophysical and geodetic monitoring due to limited local resources and occasional constraints on field accessibility, which can affect instrument installation, maintenance, and rapid response, delaying situational awareness and complicating decision-making. This study emphasizes the essential role of collaborative partnerships and new international scientific projects, including shared remote-sensing initiatives, expanded seismic and geodetic networks, technical training, and open-data frameworks, in bridging monitoring gaps, improving early-warning and emergency-response capabilities, and building long-term resilience in Ethiopia’s data-poor and resource-constrained rift environments.

How to cite: Lewi, E., Temtime, T., Biggs, J., Ayele, A., Wright, T., Pagli, C., Keir, D., and Loughlin,, S.: Seismo-Volcanic Crises Across the Red Sea and East African Rifts: The Critical Role of New Projects and International Collaborations in Data-Poor Regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1296, https://doi.org/10.5194/egusphere-egu26-1296, 2026.

EGU26-9238 | ECS | Posters on site | GI4.4

Development of a Surface Reflectance Consistency Algorithm between KOMPSAT-3A and Sentinel-2A/Landsat Satellites 

Sieun Song, Dohee Han, Sungu Lee, Jeongho Lee, Seungtaek Jeong, and Jongmin Yeom

Surface reflectance consistency of multi satellite optical satellites is an essential factor for quantitative Earth observation and multi-satellite data integration. However, due to differences in spectral response functions (SRFs), band definitions, and preprocessing strategies, surface reflectance discrepancy between satellite sensors still exists.

In this study, the surface reflectance data of Korea Multi-Purpose Satellite (KOMPSAT)-3/3A were analyzed together with Sentinel-2 MSI, Landsat-8/9 OLI, MODIS, and New-space Earth Observation Satellite (NEONSAT) data. In order to minimize the influence of surface characteristics, radiometrically stable Pseudo-Invariant Calibration Sites (PICS), including desert areas and the North Pacific Ocean (NPO), were selected.

Before performing the surface reflectance consistency analysis, sensor-dependent reflectance differences were analyzed using spectral response functions (SRFs) based on the USGS Spectral Library. Spectral differences between sensors were evaluated by simulating band-equivalent reflectance through convolution of established hyperspectral surface reflectance spectra, including the USGS Spectral Library Version 7, with the spectral response function (SRF) of each sensor. Based on these simulation results, the Spectral Band Adjustment Factor (SBAF) was calculated by applying the median-based ratio method and the regression method constrained to pass through the origin. The calculated SBAF was evaluated using SRF-based simulated reflectance, and differences in reflectance between sensors before and after adjustment were quantitatively compared and analyzed using statistical indicators such as mean, standard deviation, and RMSE.

Surface reflectance differences showed sensor- and band-dependent patterns, with more evident deviations appearing in the near-infrared (NIR) region compared to other spectral bands. Based on the SRF-based SBAF evaluation, agreement among sensors generally increased, while the degree of improvement varied depending on the spectral band and adjustment strategy, resulting in residual discrepancies in some cases. Overall, these observations summarize the present characteristics of surface reflectance differences observed between KOMPSAT and other optical satellite sensors.

In future studies, the selected PICS will be used to apply radiative transfer model–based atmospheric correction using the 6S model, in order to further assess and improve surface reflectance consistency across multiple optical satellite sensors.

This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT)(RS-2025-00515357).

How to cite: Song, S., Han, D., Lee, S., Lee, J., Jeong, S., and Yeom, J.: Development of a Surface Reflectance Consistency Algorithm between KOMPSAT-3A and Sentinel-2A/Landsat Satellites, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9238, https://doi.org/10.5194/egusphere-egu26-9238, 2026.

EGU26-11371 | Orals | GI4.4

Monitoring of Sea State and Surface Currents in Rural Coastal Areas 

Ilaria Catapano, Gianluca Gennarelli, Giuseppe Esposito, Carlo Noviello, Francesco Soldovieri, and Giovanni Ludeno

Rural coastal areas are among the most poorly monitored environments, despite being highly exposed to marine hazards, climate variability, and increasing anthropogenic pressure. Limited accessibility, the absence of permanent infrastructures, and high operational costs often prevent the deployment of conventional in situ monitoring instruments, leading to significant observational gaps in the estimation of sea state parameters and surface current dynamics. Developing sustainable and low-impact observational strategies is therefore crucial to improve environmental monitoring and risk awareness in these marginal coastal regions [1].

Satellite-based remote sensing systems provide valuable large-scale observations of ocean dynamics. However, their low revisit time and reduced performance in nearshore and shallow-water environments limit their effectiveness along rural coastlines. As a result, increasing attention has been devoted to sensing technologies operating at local scales and closer to the sea surface, including radar and video-based monitoring systems. Among radar-based solutions, short range (SR) K-band systems are particularly suited for this purpose. Their compact size, low power emissions, high temporal resolution, and sensitivity to short surface waves make them ideal for monitoring coastal and semi-enclosed environments. Moreover, recent developments in portable K-band radar prototypes enable rapid and non-invasive deployment in remote coastal areas, without the need for permanent installations [2], [3].

With regard to video monitoring, small unmanned aerial systems equipped with lightweight optical cameras have attracted considerable interest as highly flexible and cost-effective tools for rapid data acquisition in hard-to-reach areas, such as rocky coastlines, wetlands, river mouths, and sparsely populated shores [4], [5].

Within this framework, this contribution reviews the results of lightweight portable SRK-band radar for sea monitoring and presents an innovative signal processing strategy for extracting quantitative information on sea state parameters and surface current fields from drone-based optical camera. Both the considered technologies are useful for nearshore zone, where other observational systems are often unreliable or unavailable.

[1] P. Neill and M. R. Hashemi, “In situ and remote methods for resource characterization,” in E-Business Solutions, Fundamentals of Ocean Renewable Energy, S. P. Neill and M. R. Hashemi. New York, NY, USA: Academic, 2018, pp. 157–191.

[2] Ludeno, G.; Catapano, I.; Soldovieri, F.; Gennarelli, G. Retrieval of sea surface currents and directional wave spectra by 24 GHz FMCW MIMO radar. IEEE Trans. Geosci. Remote Sens. 2023, 61, 5100713.

[3] Ludeno, G.; Antuono, M.; Soldovieri, F.; Gennarelli, G. A Feasibility Study of Nearshore Bathymetry Estimation via Short-Range K-Band MIMO Radar. Remote Sens. 2024, 16, 261

[4] Streser, R. Carrasco, and J. Horstmann, “Video-based estimation of surface currents using a low-cost quadcopter,” IEEE Geosci. Remote Sens. Lett., vol. 14, no. 11, pp. 2027–2031, Nov. 2017.

[5] Solodoch, Y. Toledo, V. Grigorieva and Y. Lehahn, "Retrieval of Surface Waves Spectrum From UAV Nadir Video," IEEE Trans. Geosci. Remote Sens., vol. 63, pp. 1-14, 2025, Art no. 4201914, doi: 10.1109/TGRS.2025.3536378.

How to cite: Catapano, I., Gennarelli, G., Esposito, G., Noviello, C., Soldovieri, F., and Ludeno, G.: Monitoring of Sea State and Surface Currents in Rural Coastal Areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11371, https://doi.org/10.5194/egusphere-egu26-11371, 2026.

Unmanned Aerial Vehicles (UAVs) have become vital tools for environmental monitoring and disaster response, particularly in remote regions where ground-based infrastructure is sparse (Erdelj et al., 2017). Yet the practical value of these platforms depends heavily on precise flight control when navigating challenging terrain or conducting time-sensitive surveys after natural hazards. Tuning Model Predictive Control (MPC) weight matrices for such varied operational demands remains tedious and expertise-intensive, which slows deployment during crises.

We present an adaptive control framework merging reinforcement learning with formal stability guarantees. A learning agent tunes controller gains online while Lyapunov-based bounds confine every candidate gain to a provably stable region (Christofides et al., 2011). A projection operator acts as a hard safety layer, clipping any out-of-bounds gain before it reaches the MPC solver. The resulting architecture preserves guaranteed stability regardless of policy network behaviour—essential when aircraft operate beyond visual line of sight in poorly monitored areas.

Validation spans four UAV platforms covering a 200-fold mass range (27 g to 5.5 kg). On an aggressive 3D figure-8 trajectory (±4.0 m on both horizontal axes), tracking improves by 22–27 %. Position root mean square error falls from 0.45–0.55 m to 0.33–0.43 m, with variance reductions of 28–33 %. Across 60 evaluation trials, no stability violations occurred. Sequential transfer learning cuts per-platform training by 75 %, valuable when field crews must swap vehicles mid-campaign—switching, for instance, from a compact quadrotor on initial reconnaissance to a heavier hexacopter carrying hyperspectral sensors.

These results show that rigorous stability guarantees and learning-based adaptation can coexist. For observation campaigns in areas lacking ground-based networks, self-tuning controllers that never risk unstable flight could meaningfully extend what small drone fleets achieve—whether assessing earthquake damage or inspecting infrastructure in informal settlements.

 

References

Christofides, P.D., Liu, J., Muñoz de la Peña, D. (2011). Lyapunov-Based Model Predictive Control. In: Networked and Distributed Predictive Control. Advances in Industrial Control. Springer, London.

Erdelj, M., Natalizio, E., Chowdhury, K.R., Akyildiz, I.F. (2017). Help from the sky: Leveraging UAVs for disaster management. IEEE Pervasive Computing, 16(1), 24–32.

How to cite: Khan, A. M. and Tessema, T.: Stable Adaptive Flight Control for Multi-Platform UAV Monitoring: Combining Reinforcement Learning with Lyapunov-Guaranteed Gain Tuning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11383, https://doi.org/10.5194/egusphere-egu26-11383, 2026.

EGU26-15312 | ECS | Orals | GI4.4

Enhancing the Assessment of Historic Masonry Walls Using Multi-Frequency GPR Attribute Analysis 

Saeed Parnow, Francesco Soldovieri, Elikem Doe Atsakpo, and Fabio Tosti

The structural condition of historic masonry walls plays a crucial role in the conservation and management of cultural heritage assets. Moisture ingress, material degradation, and hidden internal defects often develop beneath the surface, remaining undetected by visual inspection alone. Traditional invasive inspection methods are limited by their local nature and the potential risk of damaging heritage fabric. Consequently, non-destructive testing (NDT) techniques capable of providing reliable subsurface information are essential.

Ground Penetrating Radar (GPR) has become a widely adopted non-destructive and cost-effective technique for investigating masonry structures [1-3], allowing the identification of internal heterogeneities, voids, and moisture-related anomalies. However, the interpretation of conventional GPR sections is frequently affected by signal complexity, non-uniqueness, and ambiguity, particularly when dealing with heterogeneous historic materials and varying wall thicknesses.

This study presents a multi-frequency GPR survey conducted on a historic brick masonry wall located in Walpole Park (Ealing, London, UK), a site of special historic interest. The primary objective was to assess the internal condition of the wall and investigate suspected moisture ingress. Data were acquired using ground-coupled GPR systems operating at 2 GHz and 600 MHz, including dual-polarised configurations (HH and VV), allowing a comparative evaluation of resolution and penetration depth for walls of approximately 25 cm and 55 cm thickness.

To enhance data interpretation, attribute analysis, originally developed in seismic exploration, was applied to the GPR datasets. Attributes such as Centroid Frequency (CF) and Instantaneous Frequency (IF) were extracted from both processed and unprocessed radar data. These attributes provide additional information on material properties and signal attenuation, which are strongly linked to moisture content, material heterogeneity, and structural condition. Three-dimensional visualisation of attribute volumes was employed to better delineate spatial variations within the masonry fabric.

Attribute-based representations significantly improved the clarity and interpretability of subsurface anomalies compared to conventional amplitude-based GPR images.

The findings confirm that GPR attribute analysis enhances the assessment of historic masonry structures and supports more reliable interpretation of moisture-related and structural features. The proposed workflow offers a robust, non-invasive tool for heritage conservation and condition monitoring, with potential for wider application across cultural heritage and built-environment diagnostics.

Keywords: Ground Penetrating Radar (GPR); Cultural Heritage; Masonry Inspection; Moisture Ingress; Signal Attribute Analysis

 

References

[1] Sambuelli, L., Bohm, G., Capizzi, P., Cardarelli, E., & Socco, L. V. (2011). The use of ground penetrating radar and complementary NDT techniques for the diagnostic of masonry structures. Near Surface Geophysics, 9(5), 433–447.

[2] Bianchini Ciampoli, L., Parnow, S., Tosti, F., and Benedetto, A.: Retrieving signs of buried historical road tracks by GPR data processing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16105, https://doi.org/10.5194/egusphere-egu25-16105, 2025.

[3] Catapano, I, Gennarelli, G., Ludeno, G., and Soldovieri, F., Applying Ground-Penetrating Radar and Microwave Tomography Data Processing in Cultural Heritage: State of the Art and Future Trends. IEEE Signal Processing Magazine, vol. 36, no. 4, pp. 53-61, July 2019, doi: 10.1109/MSP.2019.2895121. 

How to cite: Parnow, S., Soldovieri, F., Doe Atsakpo, E., and Tosti, F.: Enhancing the Assessment of Historic Masonry Walls Using Multi-Frequency GPR Attribute Analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15312, https://doi.org/10.5194/egusphere-egu26-15312, 2026.

EGU26-15507 | ECS | Posters on site | GI4.4

A Sustainability Matrix Framework for Translating Earth Observation and NDT Data into SDG-aligned Resilience and Decision-Making 

Javed Mohammad, Tesfaye Tessema, Fabio Tosti, and Laden Husamaldin

This study explores the capabilities of non-destructive testing (NDT) and Earth Observation (EO) not only as measurement technologies but as an evidence translation layer between technical data and sustainability governance. While remote sensing and NDT generate increasingly rich data on urban and coastal environments, a persistent gap remains between these data and the formats, categories, and narratives required for policy, regulation, and organisational reporting [1]. The main aim of this study is to address that gap by developing a sustainability matrix framework that structures, interprets, and reformulates NDT and EO outputs to enable meaningful use in decision-making and sustainability [2]. The matrix also provides accountability processes aligned with the United Nations Sustainable Development Goals (SDGs) [3].

The framework is illustrated through three exemplary case studies strategically spanning the built, natural and heritage environments. These are: analysing land surface temperature patterns across parks and built-up areas (SDG 13); monitoring urban green infrastructure using LiDAR and satellite imagery (SDG 15); and detecting coastal landform change with implications for heritage assets (SDG 11). The applications demonstrate how non-invasive, data-intensive methods provide spatially and temporally resolved evidence on environmental and infrastructural change (SDG 9). The core contribution, however, lies in how these results are translated into decision-relevant indicators and interpretive narratives that align with the UN 2030 Agenda for Sustainable Development [3, 4].

This research shows how technical findings become intelligible and usable for organisations, policymakers, and stakeholders concerned with risk, performance, and long-term resilience. The proposed translation layer provides a replicable approach to embedding environmental factors across planning, asset management, and regulatory contexts. It will provide an evidence base in situations where existing assessment practices are fragmented, inconsistent, or insufficient to meet emerging transparency and disclosure expectations [5, 6].

 

Keywords: Sustainability Matrix Framework; SDG Mapping; Earth Observation & NDT Integration; Resilience Decision-Making; Multi-Domain Monitoring

References

[1] Tosti, F. (2025) ‘Year III: The NDT—Journal of Non-Destructive Testing 2025 End-of-Year Editorial’, NDT, 4(1), p. 3. Available at: https://doi.org/10.3390/ndt4010003.

[2] Elliott, B. and Elliott, J. (2022) ‘Integrated reporting: sustainability, environmental and social’, in Financial Accounting and Reporting. 20th ed. Harlow, UK: Pearson Education Limited.

[3] Tsalis, T.A. et al. (2020) ‘New challenges for corporate sustainability reporting: United Nations’ 2030 Agenda for sustainable development and the sustainable development goals’, Corporate Social Responsibility and Environmental Management, 27(4), pp. 1617–1629. Available at: https://doi.org/10.1002/csr.1910.

[4] United Nations (2015) Transforming our world: the 2030 Agenda for Sustainable Development.

[5] Lai, A. and Stacchezzini, R. (2021) ‘Organisational and professional challenges amid the evolution of sustainability reporting: a theoretical framework and an agenda for future research’, Meditari Accountancy Research, 29(3), pp. 405–429. Available at: https://doi.org/10.1108/MEDAR-02-2021-1199.

[6] Financial Conduct Authority (FCA) (2022) Sustainability Disclosure Requirements (SDR) and investment labels. London. Available at: www.fca.org.uk/cp22-20-response-form.

How to cite: Mohammad, J., Tessema, T., Tosti, F., and Husamaldin, L.: A Sustainability Matrix Framework for Translating Earth Observation and NDT Data into SDG-aligned Resilience and Decision-Making, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15507, https://doi.org/10.5194/egusphere-egu26-15507, 2026.

Agro-pastoral communities in East Africa are increasingly affected by recurrent natural hazards, particularly drought, which leads to severe pasture degradation and substantial losses of livestock—their primary livelihood asset. These challenges highlight the urgent need for adaptive livelihood diversification strategies that reduce dependence on climate-sensitive resources. Beekeeping has emerged as a viable and climate-resilient alternative; however, its successful implementation requires reliable information on suitable habitats and forage availability. Advances in remote sensing and geospatial technologies provide powerful tools to support such strategies by integrating multi-source satellite data to monitor vegetation dynamics, landscape structure, and climate variability, thereby enabling informed planning and sustainable livelihood development in agro-pastoral environments. This study presents an integrated geospatial assessment of honey bee habitat suitability, fragmentation dynamics, and climate-smart apiary site selection in Yabelo (Ethiopia) and Taita-Taveta County (Kenya). Using Google Earth Engine, multi-source satellite data, including Planet Scope, Sentinel-1 SAR, Sentinel-2 multispectral imagery, and SRTM Digital Elevation Model were analyzed to map honey bee habitats through advanced machine learning techniques. Four classifiers (Gradient Tree Boosting, Random Forest, Classification and Regression Trees, and Support Vector Machine) were evaluated and combined using an Ensemble Learning Approach, achieving the highest classification accuracy, significantly outperforming individual models.

To understand landscape structure and resource accessibility, habitat fragmentation was assessed using key landscape metrics (Shannon diversity, contagion, and splitting index) across multiple spatial scales (500–3000 m buffers). Results reveal pronounced scale-dependent fragmentation, with Yabelo characterized by high landscape heterogeneity but increasing patch disconnection at larger scales, while Taita-Taveta exhibits more continuous but less diverse habitats. Human-induced land-use changes and edge effects were identified as major drivers of fragmentation, with wetlands and water bodies being particularly vulnerable.

To support adaptive beekeeping under climate change, fuzzy Multi-Criteria Decision-Making methods incorporating current and future climate projections (SSP1-2.6 and SSP5-8.5) were applied for apiary site suitability analysis. Findings indicate a projected decline in highly suitable apiary areas under future climate scenarios, highlighting climate-driven shifts in bee forage availability. Overall, this integrated framework demonstrates how ensemble machine learning, landscape ecology, and climate projections can support evidence-based, climate-resilient planning for sustainable beekeeping in East Africa.

Keywords: Agro-pastoral livelihoods, Remote sensing, Honey bee habitat, Climate change, Ensemble learning, Apiary suitability

How to cite: Walle, F. M.: An Integrated Geospatial Framework for Climate-Resilient Honey Bee Habitat Mapping, Fragmentation Assessment, and Apiary Site Selection., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16057, https://doi.org/10.5194/egusphere-egu26-16057, 2026.

EGU26-16485 | ECS | Orals | GI4.4

Immersive Auralisation (IA-XR): Visualising and Communicating Acoustic Data from Cultural Heritage Structures via Extended Reality Technology 

Elikem Doe Atsakpo, Eugenio Donati, Nicolò Squartini, Luca Bianchini Ciampoli, Tesfaye Tessema, Stephen Uzor, and Fabio Tosti

Heritage structures are widely recognised as irreplaceable cultural assets that connect communities with their history, and their preservation serves both current and future generations [1, 2]. As definitions of heritage have expanded to include tangible and intangible values and a broad range of stakeholders, conservation and refurbishment approaches aim to safeguard heritage significance by protecting material authenticity, cultural values, structural integrity, functional performance, and use.

In specific heritage spaces such as religious buildings and theatres, the acoustic environment plays a central role in cultural practices, symbolic meaning, and functional performance, making acoustics an integral component of aural heritage. Recent works in archeoacoutics highlight growing interest in a multisensory, sound-focused approach to heritage communication and interpretation. Since auditory perception is observer-centred and inherently spatial, effective communication of acoustic or aural heritage requires spatially representative, immersive media such as auralisation and extended reality (XR), which can reproduce listener-centric sound fields rather than purely visual reconstructions [3, 4].

This study thus investigates a stakeholder-centred framework for the visualisation and communication of acoustic data from heritage architecture, using immersive technologies to support the maintenance and preservation of archeoacoustic information. A three-dimensional digital model of the Roman Theatre at Palmyra, Syria, a UNESCO World Heritage Site, was refined, and room-acoustic simulations were conducted to generate auralisations representing the theatre’s acoustic performance under different listener and source configurations. These simulated acoustic outputs were integrated into an extended reality (XR) environment, enabling interactive exploration of the theatre’s acoustic characteristics through combined audio–visual–spatial representations of sound.

This immersive, auralised, interactive system is designed to support stakeholder-centred evaluation and knowledge exchange, thereby informing its refinement in relation to visualisation, interpretation, and decision-making needs.

Keywords: Auralisation; Extended Reality; Archeoacoustics; Human-in-the-loop

 

Acknowledgements: This research was funded by the Vice-Chancellor’s PhD Scholarship at the University of West London.

 

References

[1] T. Penjor, S. Banihashemi, A. Hajirasouli and H. Golzad, "Heritage building information modeling (HBIM) for heritage conservation: Framework of challenges, gaps, and existing limitations of HBIM," Digital Applications in Archaeology and Cultural Heritage, vol. 35, -07-29. 2024.

[2] J. Mu, T. Wang and Z. Zhang, "Research on the Acoustic Environment of Heritage Buildings: A Systematic Review," Buildings, vol. 12, -11-11. 2022.

[3] V. Hohmann, R. Paluch, M. Krueger, M. Meis and G. Grimm, "The Virtual Reality Lab: Realization and Application of Virtual Sound Environments," 2020.

[4] C. Innocente, L. Ulrich, S. Moos and E. Vezzetti, "A framework study on the use of immersive XR technologies in the cultural heritage domain," Journal of Cultural Heritage, vol. 62, pp. 268, -06-15. 2023.

How to cite: Doe Atsakpo, E., Donati, E., Squartini, N., Bianchini Ciampoli, L., Tessema, T., Uzor, S., and Tosti, F.: Immersive Auralisation (IA-XR): Visualising and Communicating Acoustic Data from Cultural Heritage Structures via Extended Reality Technology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16485, https://doi.org/10.5194/egusphere-egu26-16485, 2026.

EGU26-16574 | Orals | GI4.4 | Highlight

User- and Data-Centric GeoAI for Scalable Mapping  of Deprived Urban Areas: The IDEAtlas Approach for SDG 11.1.1 Monitoring 

Monika Kuffer, Bedru Tareke, Claudio Persello, Raian V. Maretto, Jon Wang, Angela Abascal, and Hector Antonio Vazquez Brust

Up-to-date spatial information on deprived urban areas (DUAs) is essential for evidence-based urban policy and for monitoring Sustainable Development Goal (SDG) indicator 11.1.1 on slums and informal settlements. Yet, many cities in low- and middle-income countries (LMICs) lack reliable, spatial data on the location, extent, and dynamics of settlements. The IDEAtlas project addresses this gap by combining Earth Observation (EO), artificial intelligence (AI) (here referred to as GeoAI), and a user-centred design framework to deliver scalable, transparent, and policy-relevant DUA maps. This is achieved through a data-centric AI approach utilizing multi-modal EO inputs, primarily Sentinel-2 multispectral imagery, supplemented by ancillary geospatial layers such as building density, topography, and proximity to infrastructure. These datasets are fused within a lightweight Multi-Branch Convolutional Neural Network (MB-CNN) architecture (~33,000 parameters) designed for efficient, city-scale processing of Sentinel data. The model produces two main outputs at 10 m resolution, which are resampled to 100 m to protect vulnerable groups: (1) binary maps of deprived urban area extent and (2) a continuous deprivation severity index building on the IDEAMAPS Domain of Deprivation Framework. Multi-temporal processing provides annual DUA maps (2019–2023), capturing settlement expansion, densification, eviction, and upgrading dynamics. Thus, IDEAtlas adopts a user- and data-centric GeoAI approach. Through Living Labs in eight pilot cities (Nairobi, Lagos, Mumbai, Jakarta, Salvador, Medellín, Mexico City, and Buenos Aires), and an ongoing expansion to a larger number of Latin American cities, local governments, national statistical offices, NGOs, and community groups co-design data needs, validated outputs, and contributed to the creation of reference data. The interactive web-based IDEAtls Portal allows users to inspect model predictions, digitise settlement boundaries, correct misclassifications, and provide contextual feedback. These user-generated annotations are reintegrated into the model, improving performance and trust. In several cities, stakeholder-driven refinement increased F1-scores by up to 13%, demonstrating the value of participatory data curation in complex urban environments.

The IDEAtlas outputs provide several policy-relevant indicators, such as total DUA area, population living in deprived areas, and temporal change metrics directly linked to SDG 11.1.1. By integrating scalable GeoAI methods with user-in-the-loop validation and open-source infrastructure, IDEAtlas demonstrates how user- and data-centric GeoAI can bridge urban data gaps. The approach strengthens local capacity, enhances transparency, supports inclusive and evidence-based urban policy, and outlines a pathway towards a transferable framework for global SDG 11.1.1. monitoring.

 

How to cite: Kuffer, M., Tareke, B., Persello, C., Maretto, R. V., Wang, J., Abascal, A., and Vazquez Brust, H. A.: User- and Data-Centric GeoAI for Scalable Mapping  of Deprived Urban Areas: The IDEAtlas Approach for SDG 11.1.1 Monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16574, https://doi.org/10.5194/egusphere-egu26-16574, 2026.

EGU26-16661 | ECS | Orals | GI4.4

Multi-year Satellite Observations Reveal Permanent Seasonal and Ephemeral Surface-water Regions in Arid and Semi-arid Areas Within the East African Region 

Atiyeh Ardakanian, Filagot Mengistu, Elias Lewi, Fabio Tosti, and Tesfaye Tessema

Surface water in semi-arid and arid regions has been adversely affected by climate change, compounded by their inherent environmental conditions. One such area is East Africa, which consists of small reservoirs, pans, and non-perennial rivers that provide critical water resources for people, livestock, and ecosystems [1]. However, these water resources are poorly monitored and highly variable in space and time. Recent global water products overlook small and ephemeral water bodies due to the spatial resolution of the satellite data used and the target scale [2]. This monitoring gap is particularly consequential because pastoral adaptation in the region is tightly shaped by the timing and distribution of water; socio-ecological studies emphasise that tracking environmental variability is essential for understanding how mobility patterns respond to climate change [3]. Remote sensing techniques offer a way to address this gap by identifying changes in water systems, including the emergence and disappearance of temporary water bodies. The objective of this study is to develop a framework that facilitates understanding of the spatial and temporal patterns of these water bodies, providing a foundation for subsequent analyses of pastoral nomadic movements and resource-use dynamics. Here, we present a multi-year monitoring framework that integrates Sentinel-1 SAR and Sentinel-2 optical imagery to map surface-water dynamics.  We develop Sentinel-1/2 stacks for a monthly compositing window, derive spectral water indices, perform spectral analysis, and include topographic variables. We use a basic classifier trained on multi-year reference data and produce a 10m water mask. Further, time-series metrics for water occurrence, duration, the number of wet spells, and transition frequency are produced. The preliminary results indicate a trend in changes to the temporal surface water and the extent of permanent water bodies. The results reveal strong contrasts between permanent lakes and reservoirs, seasonal floodplains, and highly ephemeral channels and pans. A good understanding of the pattern and location of such water bodies contributes to informed support for livelihoods in the region and to sustainable water resource management.  

 

Keywords: Arid And Semi-arid; Water Resources; Remote Sensing; Pastoral Mobility; Sar; Optical Imagery; East Africa, Sentinel-1/2

 

Acknowledgements: The Authors would like thank the following trusts, charities, organisations and individuals for their generosity in supporting this project: The Lord Faringdon Charitable Trust, The Schroder Foundation, The Cazenove Charitable Trust, The Ernest Cook Trust, Sir Henry Keswick, Ian Bond, P. F. Charitable Trust, Prospect Investment Management Limited, The Adrian Swire Charitable Trust, John Swire Charitable Trust, The Samuel Storey Family Charitable Trust, The Tanlaw Foundation, and The Wyfold Charitable Trust.

 

References

[1] Sigopi M, Shoko C, Dube T. Advancements in remote sensing technologies for accurate monitoring and management of surface water resources in Africa: an overview, limitations, and future directions. Geocarto Int 2024;39:2347935.

[2] Miura Y, Shamsudduha M, Suppasri A, Sano D. A Global Multi-Sensor Dataset of Surface Water Indices from Landsat-8 and Sentinel-2 Satellite Measurements. Sci Data 2025;12:1253.

[3] Cho, M.A., Mutanga, O. and Mabhaudhi, T. Adaptation to climate change in pastoral communities: a systematic review through a social-ecological lens. International Journal of Climate Change Strategies and Management, 2025 17(1), pp.246-267.

How to cite: Ardakanian, A., Mengistu, F., Lewi, E., Tosti, F., and Tessema, T.: Multi-year Satellite Observations Reveal Permanent Seasonal and Ephemeral Surface-water Regions in Arid and Semi-arid Areas Within the East African Region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16661, https://doi.org/10.5194/egusphere-egu26-16661, 2026.

EGU26-17451 | Posters on site | GI4.4

The role of  geophysics in monitoring  urban areas 

Francesco Soldovieri and Vincenzo Lapenna

The resilience and sustainability of urban areas depend heavily on the ability to implement strategic programs for the protection and maintenance of civil infrastructure. Structural health monitoring (SHM) of transport infrastructure (e.g., tunnels, bridges, and railways) and lifeline pipelines (e.g., water and energy networks and communication systems)  is among the main pillars of urban planning [1-3]. The ability to manage and protect urban infrastructure more effectively is becoming increasingly important, considering the growing urbanization process on a global scale and the exponential increase in extreme events related to climate change. In this scenario, urban areas will be more exposed to and vulnerable to these catastrophic events, resulting in increased socio-economic costs for the maintenance of civil infrastructures. Furthermore, even minor natural events could cause damage through cascading effects in urban networks.

Another key action within the urban planning framework is the introduction of the concept of 'compact cities’. In fact, there is a growing interest in creating spaces that accommodate multiple urban functions and services within proximity, thereby reducing the environmental footprint of urban areas and contributing to reduced energy consumption. Compact cities avoid the problems associated with urban sprawl and are an effective way of adapting to climate change. Once again, the organization of compact cities requires modern, innovative systems for managing civil infrastructures. Smart monitoring is even more important in suburban areas and remote areas, as it enables the concept of inclusivity for the populations living in these areas.

In this scenario, applied geophysics, also known as near-surface geophysics, can significantly support a wide range of urban planning activities. This work focuses on electromagnetic imaging methods widely used in urban geophysics and civil engineering.  In fact, the development of cost-effective, user-friendly sensor arrays, robust methodologies for tomographic data inversion, and AI-based and machine learning techniques has rapidly transformed these methods. Prospectives for development are identified in terms of using soft robot technologies, miniaturized sensors, and AI-based methods to acquire, process, and interpret data, as well as to design smart operational guidelines for infrastructure management, which will be presented at the conference.

 

 

  • Cuomo, V.; Soldovieri, F.; Bourquin, F.; El Faouzi, N.E.; Dumoulin, J. The necessities and the perspectives of the monitoring/surveillance systems for multi-risk scenarios of urban areas including COVID-19 pandemic. In Proceedings of the 2020 TIEMS Conference, Citizens and Cities Facing New Hazards and Threats, Oslo, Norway.
  • Soldovieri, F.; Dumoulin, J.; Ponzo, F.C.; Crinière, A.; Bourquin, F.; Cuomo, V. Association of sensing techniques with a designed ICT architecture in the ISTIMES project: application example with the monitoring of the Musmeci bridge. EWSHM 2014, 7th European Workshop on Structural Health Monitoring, Nantes, France, 8 - 11 July 2014.
  • Cuomo, V.; Soldovieri, F.; Ponzo, F.C.; Ditommaso, R. A holistic approach to long term SHM of transport infrastructures. Emerg. Manag. Soc. (TIEMS), 2018, 33, 67–84.).

How to cite: Soldovieri, F. and Lapenna, V.: The role of  geophysics in monitoring  urban areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17451, https://doi.org/10.5194/egusphere-egu26-17451, 2026.

EGU26-17691 | Posters on site | GI4.4

A Self-Developed Low-Cost Automated Soil Gas Flux System for Real-Time Monitoring: Design and Field Validation 

Ching-Chou Fu, Kuo-Hang Chen, Chin-Shang Ku, and Kuo-Wei Wu

High-frequency and long-term measurements of soil gas fluxes are essential for quantifying terrestrial carbon cycling and for monitoring fluid migration processes associated with hydrological, tectonic, and volcanic activity. However, the widespread application of automated soil gas flux observations remains limited by the high cost, power consumption, and operational complexity of commercial systems.

We present a self-developed, low-cost automated soil gas flux (ASF) system designed for real-time, long-term field monitoring. The system is based on a closed-chamber circulation concept integrating a low-cost NDIR CO₂ sensor, controlled gas mixing and flushing, humidity regulation using a drying module, and environmental correction for soil temperature and atmospheric pressure. A modular hardware architecture, combined with a microcomputer-based controller, enables flexible configuration, autonomous operation, and wireless data transmission. The system is powered by a solar-assisted lithium battery unit, allowing continuous deployment in remote environments.

Laboratory validation shows that CO₂ concentrations measured by the ASF system exhibit excellent linearity when compared with a high-precision cavity-enhanced gas analyzer (LGR M-GGA-918), with deviations generally within ±5% across a wide concentration range. Field deployments lasting more than three months demonstrate stable system performance, energy autonomy, and the ability to resolve high-temporal-resolution variability in soil CO₂ fluxes. A dedicated data-processing workflow is implemented to identify stable accumulation intervals and convert high-frequency concentration time series into instantaneous and diel-scale fluxes.

The ASF system provides a cost-efficient, scalable, and reproducible solution for continuous soil gas flux monitoring. Its open and modular design makes it suitable for applications ranging from ecosystem carbon exchange and ecohydrological studies to fault-zone degassing and volcano-related gas monitoring, and facilitates integration into multi-parameter geophysical and geochemical observation networks.

How to cite: Fu, C.-C., Chen, K.-H., Ku, C.-S., and Wu, K.-W.: A Self-Developed Low-Cost Automated Soil Gas Flux System for Real-Time Monitoring: Design and Field Validation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17691, https://doi.org/10.5194/egusphere-egu26-17691, 2026.

EGU26-19572 | Posters on site | GI4.4

BLUE-HeArTS: BLUE Heritage through Art, Technology, and Science 

Fabio Tosti, Ilaria Catapano, Atif Mohammed Ghani, David Daou, Sebastiano D'Amico, Alba Lastorina, Neil Linford, Moein Motavallizadeh Naeini, and Tesfaye Tessema

The BLUE-HeArTS project establishes a UK and EU multidisciplinary partnership and supports the development of a major Horizon Europe Pillar 2 project proposal for the call HORIZON-CL2-2026-01-HERITAGE-01: “Artistic intelligence” (Focus 2). The project employs the transformative power of the arts to address complex societal challenges, enhance soft skills and promote innovation and competitiveness.

BLUE-HeArTS integrates artistic creativity, advanced sensing technologies, and cultural heritage research into a unified framework that addresses climate-driven risks to heritage assets within the “Blue Environment”, i.e., coastal, riverine, and subterranean water systems. By embedding artists as active partners, the project translates scientific data from non-invasive sensing technologies and climate modelling, into storytelling and extended reality (XR) experiences that inspire creativity, empathy, and public engagement.

A central component of the project’s strategy is the evaluation of potential pilot demonstrators, with sites such as the Reculver Tower in Kent, UK, identified as illustrative case studies. The project proposes to explore the application of satellite monitoring, utilising high-resolution thermal imagery, alongside climate modelling to assess heritage vulnerability. Such an approach is designed to inform prototype artistic performances, effectively bridging the gap between technical data and public perception.

BLUE-HeArTS key objectives include:

  • Identifying real-world case studies in UK, Italy, and Malta as pilot demonstrators for narrative technologies to be further developed in the Horizon Europe project.
  • Designing a simplified XR-based prototype to test the effectiveness of scientific content interpreted through artistic perspectives.
  • Engaging partners, including policymakers and social sciences/humanities experts, to explore the historical, cultural, and environmental complexity of the selected sites.
  • Developing and refining the Horizon Europe proposal.

Ultimately, BLUE-HeArTS demonstrates that human-centered, art-driven innovation is essential for promoting cultural resilience. By linking technology and culture, the project ensures heritage research is inclusive and resilient to climate change.

 

Acknowledgements

The Authors would like to acknowledge the project BLUE-HeArTS (January – September 2026), funded by the British Academy under the "Pump Priming Collaboration between UK and EU Partners 2026" programme (Award Reference: PPHE26\100311).

How to cite: Tosti, F., Catapano, I., Ghani, A. M., Daou, D., D'Amico, S., Lastorina, A., Linford, N., Motavallizadeh Naeini, M., and Tessema, T.: BLUE-HeArTS: BLUE Heritage through Art, Technology, and Science, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19572, https://doi.org/10.5194/egusphere-egu26-19572, 2026.

The new generation of high-resolution nightlight sensors (e.g., SDGSat-1, Jilin-1) with a spatial resolution of 10 m and below can capture the spatial patterns and light colours of Artificial Light at Night (ALAN). Our research leverages these new generations of high spatial and spectral resolution nightlight images and in situ data collection by citizen science and through nightlight mobile applications to accurately assess electricity access and reliability in Sub-Saharan African cities. More than 50% of Sub-Saharan Africa’s population (around 600 million people) has no access to electricity, and a large part (estimated at 80%) does not have access to stable electricity- data coming from the global dataset "Global Electrification Project" (World Bank). Existing global electricity access datasets use low-resolution satellite data (such as VIIRS) and, therefore, remain uncertain and misrepresent that many of these cities have universal access to electricity. In reality, many residents lack formal grid connections and face unreliable electricity supply. We conducted local fieldwork in informal settlements to capture access gaps and relate the results to high-resolution ALAN data. Surveyed areas experiencing unstable access to electric power, leading to frequent outages, such as Nigeria's average of over 32 monthly outages. Results show that field observations in combination with high-resolution night light images can provide a more accurate and nuanced understanding of electricity distribution and reliability to understand the gaps in SDG-7 across sub-Saharan Africa. Our study provides insights into how global monitoring of the multiple dimensions of urban poverty can include access to electricity as an essential indicator. Furthermore, emphasises incorporating nighttime light observations into global urban poverty monitoring to include electricity access as an essential indicator. It also outlines the need for advanced satellite-based sensors to support comprehensive urban poverty mapping, in line with the European Space Agency-funded “NightWatch” project.

How to cite: Abascal, A., Kuffer, M., and Kyba, C.: Capturing the Urban Divide in Nighttime Light Images with the New Generation of High-Resolution Night Light Images and Citizen Science Data. , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20229, https://doi.org/10.5194/egusphere-egu26-20229, 2026.

EGU26-20426 | Posters on site | GI4.4

A smart approach for long-term SHM of critical infrastructures  

Francesco Soldovieri, Vincenzo Cuomo, Felice Ponzo, Rocco Di Tommaso, and Vincenzo Lapenna

In recent years, the development of monitoring and early warning systems for critical infrastructures has become increasingly relevant, as highlighted by the scientific literature and the significant number of projects focused on this specific topic, as well as their practical applications.

In this frame, the necessity arises of developing holistic approaches/strategies [1, 2], which are based not only on the integration of different sensing technologies, but more importantly on a multidisciplinary approach encompassing disciplines related to sensing, ICT, positioning technologies, and civil engineering methodologies. This contribution will provide a brief survey of the different classes of sensing techniques supporting civil engineering analysis. In addition, the other main aim of this abstract will be the setup of smart and effective observational chains for smart and sustainable monitoring, especially concerning marginal areas. Attention will also be given to the embedded miniaturized sensors, which have the main advantage of ensuring an always updated long-term monitoring and provide a more reliable early-warning system. Finally, it is evident that the concepts specifically considered here for critical infrastructures can also be extended to urban areas (built environment) and cultural heritage.

[1] Soldovieri, F.; Dumoulin, J.; Ponzo, F.C.; Crinière, A.; Bourquin, F.; Cuomo, V. Association of sensing techniques with a designed ICT architecture in the ISTIMES project: application example with the monitoring of the Musmeci bridge. EWSHM 2014, 7th European Workshop on Structural Health Monitoring, Nantes, France, 8 - 11 July 2014.

[2] Cuomo, V.; Soldovieri, F.; Ponzo, F.C.; Ditommaso, R. A holistic approach to long term SHM of transport infrastructures. Emerg. Manag. Soc. (TIEMS), 2018, 33, 67–84.).

 

How to cite: Soldovieri, F., Cuomo, V., Ponzo, F., Di Tommaso, R., and Lapenna, V.: A smart approach for long-term SHM of critical infrastructures , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20426, https://doi.org/10.5194/egusphere-egu26-20426, 2026.

In previous work, we applied a spatially-aware graph neural network model to West Nile virus data collected in Illinois for mosquito surveillance. The purpose of this was to aid mosquito abatement efforts within the state while accounting for environmental variability. Other studies have also taken this data to examine links between West Nile virus levels and spatially-varying demographic factors, but did not identify any evidence of such links. This raises the question of whether the inability to identify such links could be due to confounding via surveillance levels related to the demographic factors. That is to say, such links may be disguised by varying West Nile virus surveillance data quality across Illinois, and this variance in data quality may be related to the demographic factors themselves. In our work, we examine the spatial trends of surveillance frequency in this data within the Chicago area using a functional data analysis model within a Bayesian hierarchical model that is implemented in the Stan probabilistic programming language. We then relate these trends to zipcode-level demographic factors and present the likelihood for the existence of the statistical relationships in question. The use of a functional data analysis method allows for increased flexibility in our choice of model, such that it more closely reflects the reality supported by our sources from various fields in the literature. Furthermore, our use of a Bayesian hierarchical framework allows for greater interpretability of our findings, at the cost of greater required computational resources for model fitting.

How to cite: Tonks, A., Bravo, L., and Smith, R.: Confounding effects via spatially-varying demographic factors upon West Nile virus surveillance in Illinois identified using a Bayesian functional data analysis model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23010, https://doi.org/10.5194/egusphere-egu26-23010, 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.


Muography is a rapidly evolving interdisciplinary field that uses cosmic-ray muons to image the internal structure of large objects. Muons are highly penetrating particles whose energy loss depends on the distance traveled in a medium (e.g., rock) and on the medium’s density. By detecting and analyzing muons that pass through an object, it is possible to reconstruct its internal density distribution. This emerging method offers new opportunities in areas such as mining, volcano monitoring, cave exploration, archaeology, and structural diagnostics.

The muography project portfolio of HUN-REN Wigner Research Centre for Physics is actively engaged in developing hardware and software for muography detectors, as well as in advancing data-processing techniques and exploring potential applications. We maintain several international collaborations, within which multiple successful measurements have been conducted in active European mines.

In this presentation, we focus on muograpic measurements conducted in the Jánossy Underground Laboratory. This lab is located on the KFKI Campus in Budapest, Hungary, provides a well-characterized environment ideally suited for testing our detectors and evaluating the various steps of muography data processing. The main objective of this measurement program is to build a comprehensive dataset that supports the refinement of data processing methods, the testing of different inversion techniques, and precision parameter analysis using well-defined artificial anomalies (tunnels). We will discuss the results of a series of measurements carried out at the laboratory and the developments derived from these studies: 

- validation of the direct problem

-inversion distortion analysis and sensitivity test

-precision parameter analysis (diameter, direction, position) using known tunnels 

How to cite: Stefán, B. A., Hamar, G., Balázs, L., and Surányi, G.: Development of muography data processing and procedures, inversion and precision parameter analysis based on measurements performed at the Jánossy Underground Laboratory, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1255, https://doi.org/10.5194/egusphere-egu26-1255, 2026.

Cosmic-ray neutron sensing (CRNS) has emerged as a powerful tool for monitoring near-surface water across a wide range of spatial scales, from soil moisture and snowpack on Earth to hydrogen mapping on planetary surfaces. While most terrestrial CRNS applications focus on environments with appreciable liquid water, far less is known about neutron behavior in extremely dry systems where hydrogen is sparse and primarily bound in minerals. These conditions are directly relevant to planetary neutron spectroscopy and provide an opportunity to connect environmental CRNS research with space science.

Here we present results from portable CRNS deployments at ultra-dry terrestrial analog sites, including Alvord Desert, Oregon, and the Namib Desert, Namibia. These campaigns targeted sites spanning very dry to dry conditions, dune and interdune settings, and minimal vegetation, allowing us to examine local-scale variability in moderated and bare neutron measurements under low-moisture endmember conditions. We apply state-of-the-art corrections for atmospheric pressure, water vapor, and incoming cosmic-ray intensity, and propagate counting statistics to assess uncertainty at rover-scale and field-scale integration times.

A central motivation for this work is the interpretation of passive neutron data acquired by the Dynamic Albedo of Neutrons (DAN) instrument on the Curiosity rover following the loss of its active pulsed neutron generator. Unlike terrestrial CRNS studies, Mars lacks direct ground-truth soil moisture measurements, and near-surface liquid water or ice is unstable at equatorial latitudes. As a result, the neutron signal is dominated by mineral-bound hydrogen and bulk composition effects. The terrestrial analog sites presented here provide a controlled framework for understanding neutron sensitivity, spatial variability, and correction strategies in similarly dry environments, while leveraging active neutron measurements and in situ sensors on Earth as calibration anchors.

Our results demonstrate that even under extremely dry conditions, corrected neutron counts exhibit measurable spatial and temporal structure, and that uncertainties associated with environmental corrections can be comparable to or exceed those from counting statistics. These findings highlight the value of cross-disciplinary collaboration between planetary science and environmental CRNS communities, and suggest that dry terrestrial analogs can play a key role in improving neutron-based water detection and modeling across Earth and planetary applications.

How to cite: Hardgrove, C. and Franz, T.: Cosmic-Ray Neutron Sensing in Ultra-Dry Environments: Linking Terrestrial Mars Analogs and Planetary Neutron Spectroscopy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3177, https://doi.org/10.5194/egusphere-egu26-3177, 2026.

The need to measure soil moisture accurately and continuously and to monitor its climatic impact has moved into the public focus through the rising number of flood events and droughts in recent years. Currently the German Meteorological Service (DWD) operates a soil moisture viewer based on the soil-vegetation-atmosphere-model AMBAV and provides agrometeorological consultation. In addition to modelled soil moisture data, several institutions and some federal states started to set up their own soil moisture observations locally, but a nationwide observation network is still lacking in Germany.

The DWD’s internal project IsaBoM (“Integration of standardized and automatized soil moisture measurements in the DWD observation network”) aims to prepare the introduction of automized soil moisture measurements with two complementary measuring systems (in-situ sensors and Cosmic-Ray Neutron Sensing - CRNS), following the guidelines of the WMO (World Meteorological Organization) to permanently monitor this essential climate variable. The project’s tasks are, amongst other aspects, testing and selecting suitable sensors and calibration procedures, setting up data analysis methods, preparing the automatic dataflow and public data provisioning and ultimately providing solutions to integrate the soil moisture data into the existing operational models.

Here, we present the progress of the project IsaBoM for the preparation of a nationwide soil moisture network starting with 20 preliminary designated stations of the DWD’s operational network, where the chosen locations are representative of the soil properties and climatic conditions throughout Germany, while also being equally distributed geographically. We report on first results from our two test sites in Braunschweig and Dürnast (Freising), where the parallel measurements of multiple arrays of in-situ sensors and several CRNS sensors are tested on two operational DWD measurement sites differing in soil type and climate and providing additional meteorological measurements. We show first comparisons of soil moisture estimates from CRNS detectors with different sensitivities and the observed effects of precipitation, vegetation cover and irrigation on the signal.  The CRNS signals at both stations are calibrated using repeated soil sampling campaigns with varying equipment. Additionally, experimental sensor layouts (arrangement of in-situ profiles towards the CRNS) are used to further test the comparability and synergies between the two systems.

Feasible solutions and means for the optimal utilization of both soil moisture measuring systems, while adapting to the particular conditions when deployed on operational meteorological measurement sites, are discussed with regards to the chances and challenges from the perspective of a meteorological service.

How to cite: Albert, M., Herbst, M., Hufnagl, L., Kurtz, W., and Lenkeit, J.: Integration of in-situ and Cosmic-Ray Neutron Sensing derived soil moisture measurements into the observation network of the German Meteorological Service – progress of the project IsaBoM, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4197, https://doi.org/10.5194/egusphere-egu26-4197, 2026.

EGU26-4249 | ECS | Posters on site | GI4.7

Characterizing Multi-Timescale Soil Moisture Memory across Australia's CosmOz Network 

Nagesh Mishra, Nikhil Rajdeep, Subbarao Pichuka, Robert Faggian, and David McJannet

Memory effects are ubiquitous in geophysical systems, arising from internal dynamics and interactions with external forcings across multiple timescales. Within land surface systems, soil moisture memory is a key factor governing land–atmosphere feedbacks, influencing the intensity, persistence, and predictability of hydro-climatic extremes such as droughts and floods. This study quantifies soil moisture memory across the CosmOz-Australia network using long-term Cosmic Ray Neutron Sensing (CRNS) observations and characterizes memory across land surface and meteorological timescales.

The CRNS technique offers a novel, field-scale measurement of soil moisture with high temporal resolution and a time-varying effective sensing depth, thereby overcoming the limitations of traditional point-scale observations and enabling the robust characterization of soil moisture memory across various timescales. Despite the widespread application of CRNS data for soil moisture monitoring and validation, their potential for systematic, multi-timescale soil moisture memory estimation has not yet been explored.

This study estimates the short-term energy-limited (τs) and long-term water-limited (τL) memory components applying a hybrid stochastic-deterministic modeling framework that represents rapid surface-layer responses and slower root-zone and subsurface controls at the land surface scale. In addition, to capture memory at the meteorological scale, we estimate a non-parametric, model-free entropy-based effective memory timescale that quantifies information persistence beyond linear correlations, and compute the e-folding memory timescale as a standard measure of decorrelation. Results reveal pronounced spatial heterogeneity in soil moisture memory across Australia. Short-term memory is consistently low (median τs ≈ 0.3–1.0 days), reflecting rapid drying over the effective sensing depth and low memory in drylands. Long-term memory (median τL ≈ 4–11 days) is highest over the humid eastern and south-eastern regions, consistent with a water-limited evapotranspiration regime where higher precipitation frequency, lower aridity, finer soils, and denser vegetation enhance root-zone storage and slow anomaly decay. Entropy-based effective memory ranges from approximately 19 to 36 days, indicating substantial information retention at monthly timescales, while e-folding timescales extend up to ~70 days in temperate and monsoon-influenced regions. The strong spatial agreement between entropy-based and correlation-based metrics suggests robust and consistent soil moisture memory regimes across Australia, highlighting their dependence on hydro-climate, soil texture, and vegetation. The results provide observation-based characterization of multi-timescale soil moisture memory using CRNS data, with important implications for land surface model evaluation, drought diagnostics, and sub-seasonal to seasonal climate forecasting.

How to cite: Mishra, N., Rajdeep, N., Pichuka, S., Faggian, R., and McJannet, D.: Characterizing Multi-Timescale Soil Moisture Memory across Australia's CosmOz Network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4249, https://doi.org/10.5194/egusphere-egu26-4249, 2026.

EGU26-7994 | ECS | Orals | GI4.7

Bridging Synthetic Modeling and Field Reality: Assessing Dry-Region Dominance in Cosmic-Ray Neutron Sensing via Geophysical Integration 

Viola Cioffi, Luca Peruzzo, Matteo Censini, Mirko Pavoni, Francesca Manca, Markus Köhli, Jannis Weimar, and Giorgio Cassiani

The accurate quantification of field-scale volumetric water content (VWC) is a critical requirement across multiple disciplines, from optimizing irrigation in precision agriculture to assessing slope stability and managing regional water resources. Cosmic-Ray Neutron Sensing (CRNS) is a pivotal non-invasive technology, providing integrated VWC estimates over large footprints (10–20 hectares) and significant depths (up to 80 cm). However, the interpretation of CRNS data in heterogeneous environments remains challenging. The inherently non-linear relationship between neutron intensity and hydrogen content, combined with a complex spatial weighting function, leads to "dry-region dominance," where the sensor response is disproportionately influenced by the drier portions of the soil. This research investigates these effects through a multidisciplinary workflow that integrates CRNS monitoring with preliminary geophysical spatial characterization. The first stage involved a purely synthetic investigation using the URANOS Monte Carlo neutron transport code to replicate the subsurface heterogeneity of the Borgo Grignanello site (Siena, Italy). To ensure a controlled and quantifiable comparison, the site was represented through a simplified two-region ground model characterized by distinct VWC values, constrained by several high-resolution Electrical Resistivity Tomography (ERT) transects and Electromagnetic Induction (EMI) data. This simplified framework provided a robust "forward model" and numerical proof of the dry-region bias: the derived VWC in the heterogeneous domain demonstrated an agreement with RMSE of 1.01% with the values of the drier region.

To provide empirical evidence for these synthetic findings, the second part of the research compares real CRNS time series with local TDR sensors during selected infiltration events. Given that the local sensors are positioned within the wetter units of the site, a significant incongruence between the two datasets is observed. This discrepancy serves as a direct experimental validation of the dry-region dominance predicted by the forward model, confirming that the CRNS signal is governed by the drier soil components, which effectively overshadow the moisture values of the wetter units in such heterogeneous contexts.

In conclusion, this work demonstrates that a multidisciplinary geophysical strategy is key to a more accurate interpretation of CRNS datasets. By integrating synthetic modeling with prior site characterization, this framework provides the reliable, spatially-aware insights necessary for effective hydrological modeling, natural hazard mitigation, and sustainable land management

How to cite: Cioffi, V., Peruzzo, L., Censini, M., Pavoni, M., Manca, F., Köhli, M., Weimar, J., and Cassiani, G.: Bridging Synthetic Modeling and Field Reality: Assessing Dry-Region Dominance in Cosmic-Ray Neutron Sensing via Geophysical Integration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7994, https://doi.org/10.5194/egusphere-egu26-7994, 2026.

EGU26-8396 | Posters on site | GI4.7

Recent developments in cosmic ray soil moisture observing system in Slovenia 

Rozalija Cvejić, Martina Bavec, Matjaž Glavan, Nejc Golob, Marija Klopčič, Tamara Korošec, Matjaž Mikoš, Boštjan Naglič, Matic Noč, Urša Pečan, Tatjana Pirman, Maja Podgornik, Denis Rusjan, Špela Srdoč, Denis Stajnko, Žiga Švegelj, and Vesna Zupanc

Reliable soil moisture observations are pivotal for informing sustainable agricultural decisions under an ongoing changing climate. A cosmic-ray soil moisture observing system (SI-COSMOS) network was established for the period 2025-2040 to enhance soil moisture monitoring in Slovenia. The rationale was based on extensive experience with point soil moisture sensors in operational decision-making at the farm level, where they proved highly vulnerable to damage from land operations and wildlife activity. At the same time, the information was limited to micro-local conditions. As an alternative, a less vulnerable, non-invasive, intermediate soil-moisture network was established. As of Jan 2026, the network consists of 14 cosmic ray neutron sensors (CRNS). In this contribution, we present the network architecture, current calibration experiences, and discuss the network's role in the national and international context.

SI-COSMOS locations spread across the Continental, Alpine, Karst, Mediterranean, and Pannonian regions. Installed are lithium fluoride and boron carbide-based CRNS. The network's elevation ranges from 10 m to 500 m above sea level. Land use at locations includes olive groves (3), grasslands and pastures (2), hop plantations (2), mixed land-use systems (6), and forest (1), mainly under rainfed, but also irrigated (drip, drum, and pivot) conditions. Soil moisture is captured in various soil types.

At the national scale, the vision of SI-COSMOS is to support investigating soil–water-plant–atmosphere interactions under diverse climate, land-use, and soil conditions, to support improved drought detection and management, as well as hydrological modelling and applications. Additionally, the network aims to further develop and validate surface soil moisture products based on remote sensing or modelled data, for improved large-scale soil moisture observations at the national and international scales. Products based on SI-COSMOS will support development of transferable real-time land management tools for enhanced water resilience.

Acknowledgements: This research was funded by the Slovenian Research Agency (ARRS) with a grant to the Ph.D. students Nejc Golob and Špela Srdoč, and partially supported by research programme P4-0085, national targeted research project (V4-2406), Interreg Alpine Space program, project Alpine Space Drought Prediction (A-DROP) (grant number 101147797), European Union – LIFE Programme (LIFE23-IPC-SI-LIFE4ADAPT), OPTAIN Horizon 2020 (grant number 862756), the NextGenerationEU project ULTRA 4. Sustainable Environment, and the Slovenian CAP Strategic Plan 2023–2027.

How to cite: Cvejić, R., Bavec, M., Glavan, M., Golob, N., Klopčič, M., Korošec, T., Mikoš, M., Naglič, B., Noč, M., Pečan, U., Pirman, T., Podgornik, M., Rusjan, D., Srdoč, Š., Stajnko, D., Švegelj, Ž., and Zupanc, V.: Recent developments in cosmic ray soil moisture observing system in Slovenia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8396, https://doi.org/10.5194/egusphere-egu26-8396, 2026.

EGU26-11143 | ECS | Posters on site | GI4.7

Estimation of Spatiotemporal Soil Moisture Dynamics in a Temperate Organic Alley Cropping System in Hessen, Germany 

Alvin John Felipe, Farimah Asadi, Lutz Breuer, and Suzanne Jacobs

The exponentially growing population drives the intensification of agricultural production, which contributes to land and water quality degradation, biodiversity loss, and climate change. In this regard, nature-based solutions like silvoarable agroforestry systems, which integrate trees on arable land, have taken a new dawn due to their potential multifaceted benefits derived from nature’s contributions to people. Among the limiting factors in sustainable agricultural production is water availability, which governs biogeochemical processes, such as the regulation of material fluxes, nutrient availability and movement, carbon sequestration, microbial activity, and modification of soil properties. In temperate agroforestry systems, soil moisture regimes are not well understood. Efforts in collecting long-term data are of high importance, particularly in determining how agroforestry systems in temperate climates affect water availability and, therefore, their potential to support food production under current and future climate conditions. Knowledge of soil moisture could help in understanding whether agroforestry systems improve water availability for crop growth, which would offer resilience against droughts, or, on the other hand, cause competition with trees that reduces soil moisture availability.

In this ongoing study, we investigate point- and field-scale soil moisture dynamics in a six-year-old organic alley cropping system in Hessen, Germany. The system consists of six strips of 3-meter-wide tree rows with apple, poplar, and timber trees, alternated with 18-meter-wide crop alleys. We instrumented three transects with Frequency Domain Reflectometry (FDR) soil moisture sensors at 1, 2.5, 6, and 10.5 meters perpendicular from the tree row (upslope and downslope) at 10, 40, and 60 cm depths, to study soil moisture dynamics along the tree-crop interface. We also employed three cosmic ray neutron sensors (CRNS) to assess the field-scale trend and dynamics of the soil moisture based on the inverse relationship of the amount of hydrogen (water) in the soil and the intensity of epithermal neutrons over its dynamic footprint. Here, we present our experimental setup to capture both the transect-point scale and field-scale spatiotemporal soil moisture patterns and show preliminary findings for a full cropping season. Such an approach has the potential to provide soil moisture data at different scales relevant to efficient system design, tree-crop species selection, and agricultural water management.

How to cite: Felipe, A. J., Asadi, F., Breuer, L., and Jacobs, S.: Estimation of Spatiotemporal Soil Moisture Dynamics in a Temperate Organic Alley Cropping System in Hessen, Germany, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11143, https://doi.org/10.5194/egusphere-egu26-11143, 2026.

EGU26-11732 | Orals | GI4.7

Can Cosmic Rays Neutron Sensors provide valuable data about space weather events? 

Gianmarco Cracco, Enrico Gazzola, Martin Schrön, Roberto Salzano, Solveig Landmark, Tino Rödiger, and Andre Daccache

Cosmic Rays Neutron Sensing (CRNS) is a method to derive the amount of water in the environment by the measurement of neutron albedo in the proximity of the soil. The signal is strongly affected by the incoming cosmic rays modulation, requiring a continuous real-time correction that is typically achieved by taking as a reference the observations provided by the Neutron-Monitor DataBase (NMDB). Using the incoming flux of muons as a reference has been proposed as an alternative method of correction by Finapp, whose CRNS detector is capable of contextually measuring both neutrons and muons.

What is noise for some can be signal for others, which leads to increasing collaboration between the CRNS and the Space Weather communities. While CRNS devices cannot provide a level of accuracy and resolution comparable to dedicated neutron monitors, they would compensate with the number of deployed detectors. Being low-cost, easy to install and maintain, their use is spreading fast for various purposes, from agriculture to environmental monitoring. This can be seen as a low-cost world-wide diffuse observatory, potentially with a much higher spatial density than the NMDB and spontaneously growing.

Assessing how neutron and muon count rates measured by these devices are affected by space weather events, like Forbush decreases or Ground-Level Enhancements (GLE), could increase the understanding and monitoring of such events by providing a mapping of their impact on the Earth surface. If the CRNS station is equipped with a Finapp detector, the contextual detection of muons can provide additional information.

In this presentation we will analyze how a small set of Finapp CRNS probes, located in different locations of Earth, responded to some major events of Furbush decrease or GLE, in the neutron and muon count rate signals. The set includes, among others, two probes located in NMDB sites (OULU and JUNG) and a probe installed in Svalbard. This aims to be an example of the potential interest of CRNS for Space Weather investigation. A large database of collected data may be already available and underused.

Acknowledgement

We acknowledge the NMDB database (www.nmdb.eu), founded under the European Union's FP7 programme (contract no. 213007) for providing data. Jungfraujoch neutron monitor data were kindly provided by the Physikalisches Institut, University of Bern, Switzerland. Oulu neutron monitor data were kindly provided by the Sodankyla Geophysical Observatory (https://cosmicrays.oulu.fi). CaLMa neutron monitor data were kindly provided by the Space Research Group (SRG-UAH), University of Alcala, Spain.

How to cite: Cracco, G., Gazzola, E., Schrön, M., Salzano, R., Landmark, S., Rödiger, T., and Daccache, A.: Can Cosmic Rays Neutron Sensors provide valuable data about space weather events?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11732, https://doi.org/10.5194/egusphere-egu26-11732, 2026.

EGU26-12026 | Posters on site | GI4.7

Automated Contextual Pre-processing of Mobile Rail-CRNS Measurements for Large-Scale Soil Water Content Assessment  

Daniel Altdorff, Solveig Landmark, Steffen Zacharias, Sascha E. Oswald, Peter Dietrich, Attinger Attinger, and Martin Schrön

Soil water content (SWC) is a key variable in hydrology, agriculture, and climate research, but large-scale measurements remain challenging due to spatial heterogeneity and logistical limitations. Stationary Cosmic Ray Neutron Sensing (CRNS) provides intermediate-scale estimates (~200m footprint), yet covers only local areas. Mobile Rail-CRNS platforms overcome this by enabling continuous SWC mapping along hundreds of kilometers of railway networks. In 2024, the UFZ operated five such Rail-CRNS systems, collecting data up to hundredth of kilometer daily across diverse landscapes in Germany. However, rail roving multiplies exposure to dynamic environmental influences (e.g., tunnels, bridges, parallel tracks, urban areas, water bodies, roads, topography, biomass/forest types), which can systematically bias neutron signals. Further, inaccuracies in GPS positioning can cause the measurement positions to be several meters off the track. At this data volume, manual screening is infeasible, automated detection, flagging, and quantitative scoring of these influences are required for data quality control and correction.

Here we present a fully automated, Python-based pre-processing pipeline that evaluates measurements at both point and segment levels. GPS positions are first snapped to OSM railway tracks (nearest-points projection) to correct for localization errors. Each point is then queried for proximity to OSM features, tree species from the German Aerospace Center and DEM-derived topography, using configurable minimum feature sizes (e.g. length of a river, tunnel), influence radii, and weights (e.g., tunnel > bridge). These parameters can be flexibly adjusted and regionally adapted. To address the integral nature of mobile measurements, we introduce segment-based scoring: Intervals between consecutive points are subdivided into subsamples (minimum 3, additional every ~10 m for longer segments), incorporating direction (azimuth) for asymmetric effects (e.g., lateral slopes) guaranteeing its real length but its planar projection. Influences are evaluated proportionally. In addition, for segments above a defined length, a speed flag is added to indicate reduced data density and reliability.

An interactive map allows you to review the selected settings in relation to the potentially influencing features: Segment colors reflect its cumulative scores, flags as rings in relation to its cause, and geo-layers toggleable. Mouse-over tooltips provide instant score breakdowns for iterative parameter tuning.

The pipeline enables targeted filtering of uncertain segments, application of region- or forest-type-specific correction factors, and integrative comparison of land-use groups (point vs. segment scale). Initially tested on a pilot transect in the Harz Mountains (~ 8 km), ~60% were marked as having substantial impacts, demonstrating its necessity as well as its robustness and practical applicability. Fully transferable across Germany, it paves the way for consistent, large-scale Rail-CRNS SWC mapping. Future steps include machine-learning-based weight optimization.

 

How to cite: Altdorff, D., Landmark, S., Zacharias, S., Oswald, S. E., Dietrich, P., Attinger, A., and Schrön, M.: Automated Contextual Pre-processing of Mobile Rail-CRNS Measurements for Large-Scale Soil Water Content Assessment , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12026, https://doi.org/10.5194/egusphere-egu26-12026, 2026.

EGU26-12686 | ECS | Posters on site | GI4.7

Cosmic Ray Neutron Sensing (CRNS) as a Space Weather Tool? 

Hanna Giese, Stephan Böttcher, Bernd Heber, Konstantin Herbst, Lasse Hertle, and Martin Schrön

Since mid 2024 a CRNS detector has been installed in Kiel close to the Kiel neutron monitor (NM). The latter is a measure of the incoming cosmic ray induced neutron environment and is used to correct the CRNS data in order to determine the soil moisture in the surrounding area of the system. 
The fact that the CRNS detector and the NM are at the same location allows a unique insight into the correlation of both measurements. Since both count rates are expected to decrease during Forbush Decreases (FDs) we can investigate their correlation during all FDs observed from mid 2024. In contrast, the correlation is far lower during the occurrence of rain events, which can lead to a similar shaped decrease in the count rate. The analysis has been repeated utilizing NMs at different locations (e.g. Jungfraujoch) in order to estimate the uncertainties of the above analysis. Furthermore, the count rates of different CRNS detectors have been compared for FDs as well as rain events to see if a distinction between both is possible without the use of a NM.

How to cite: Giese, H., Böttcher, S., Heber, B., Herbst, K., Hertle, L., and Schrön, M.: Cosmic Ray Neutron Sensing (CRNS) as a Space Weather Tool?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12686, https://doi.org/10.5194/egusphere-egu26-12686, 2026.

EGU26-13972 | Orals | GI4.7

Assessing an empirical approach to derive SWE from CRNS for pre‑alpine to high‑alpine locations 

Benjamin Fersch, Nora Krebs, and Paul Schattan

When high‑energy cosmic rays strike the upper atmosphere, they produce cascades of secondary particles, including fast neutrons that reach the Earth's surface. These neutrons are efficiently moderated by collisions with hydrogen atoms; consequently, the intensity of the neutron flux above ground decreases in proportion to the amount of water present—whether stored in the soil, in liquid form, or frozen as snow.

A stationary cosmic-ray neutron sensing (CRNS) detector records counts of these epithermal neutrons, and a single local water‑content reference is sufficient to convert the count rate into a quantitative estimate of soil moisture. The count‑versus‑moisture relationship has been shown to be remarkably consistent across diverse soils, climates, and geographic regions.

Because the calibration curve is essentially universal, typically only a single in‑situ reference measurement is required; thereafter, and retrospectively, the detector can continuously monitor spatially integrated changes in soil moisture. This simplicity has established CRNS as a valuable tool for agricultural water management, hydrological research, and field‑scale climate monitoring.

In contrast, converting neutron counts to snow water equivalent (SWE) for a sensor positioned above the snowpack has required extensive site‑specific calibration, which has hindered rapid network expansion. This difficulty arises from discrepancies between theoretical models and the limited empirical data available.

Based on a compilation of extensive in‑situ measurements at several montane locations within the Pre‑Alpine Terrestrial Environmental Observatory (TERENO Pre‑Alpine), we derived a set of empirical coefficients for the count–SWE relationship. Most locations in our dataset show good agreement with these empirical coefficients, although some outliers exist. Nevertheless, this empirical approach can reduce the effort required to establish new CRNS stations for SWE monitoring. We also evaluate transferability to alpine–nival sites—characterized by shallow soils, steep topography, and very high SWE—and analyze causes of deviations in the empirical approach’s performance due to site-specific environmental conditions.

How to cite: Fersch, B., Krebs, N., and Schattan, P.: Assessing an empirical approach to derive SWE from CRNS for pre‑alpine to high‑alpine locations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13972, https://doi.org/10.5194/egusphere-egu26-13972, 2026.

EGU26-16311 | ECS | Posters on site | GI4.7

Long Short-Term Memory model to predict root zone soil water content from neutron count measured by Cosmic Ray Neutron Sensing 

Atina Umi Kalsum, Pieter Janssens, Jan Vanderborght, and Jan Diels

Accurate estimation of soil water content in the root zone (e.g., 0 – 30 cm) is essential for designing irrigation schedules and requires measurements that represent the field scale. Cosmic Ray Neutron Sensing (CRNS) offers a non-invasive solution that provides integrated soil moisture measurements with a horizontal footprint of approximately 7 to14 hectares and depths ranging from 15 to 83 cm, making it suitable in an area with a homogenous land use, like agricultural fields. However, CRNS sensitivity varies with both distance and depth relative to the sensor, complicating its use for estimating soil moisture in specific layers. When soil moisture is known, it is feasible to perform a forward calculation to derive neutron counts from soil water content. In this study, such calculations were performed using COSMIC, integrated with the HYDRUS-1D model. However, backward calculations, deriving soil water content from neutron counts, are not straightforward. This is because wetting and drying processes start at the soil surface, where CRNS is most sensitive. Consequently, the integrated measurement disproportionately reflects changes in the upper layers, creating a non-unique or hysteretic relationship between neutron counts and soil moisture during wetting and drying cycles. This makes predicting the 0 – 30 cm water content from neutron counts particularly challenging.

To address these limitations, we explore the application of the Long Short-Term Memory (LSTM) model to predict the average soil water content in the 0 – 30 cm layer by training the model using time series of average 0 – 30 cm soil water content and neutron counts (simulated with HYDRUS-1D COSMIC) as well as meteorological data (precipitation and reference evapotranspiration). The LSTM model is well-suited because it can learn temporal dependencies and patterns of long sequence data. The initial simulations were based on three years record of synthetic data under bare soil conditions for a region in Flanders, Belgium. While initial findings indicate a potential, further research will focus on improving the model’s robustness by training the model with more diverse variables, expanding the dataset, and integrating field measurement soil moisture records to enhance its applicability across different scenarios. This research highlights the feasibility of combining CRNS measurement, physically based modelling, and data-driven techniques to improve soil moisture estimation for irrigation management.

How to cite: Kalsum, A. U., Janssens, P., Vanderborght, J., and Diels, J.: Long Short-Term Memory model to predict root zone soil water content from neutron count measured by Cosmic Ray Neutron Sensing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16311, https://doi.org/10.5194/egusphere-egu26-16311, 2026.

EGU26-18160 | Posters on site | GI4.7

The SoMMet characterization of a Finapp Cosmic-Ray Neutron Sensor and its first real-world application 

Enrico Gazzola, Zdenek Vykydal, Rudi Nadalet, Martin Pernter, Roberto Dinale, Stefano Gianessi, and Barbara Biasuzzi

Cosmic Ray Neutron Sensing (CRNS) has been established as a reliable method for measuring Soil Moisture (SM) at an intermediate spatial scale, bridging the gap between point-scale measurements and satellite observations. While CRNS stations are increasingly included in meteorological and environmental monitoring networks, integration and intercomparison between different methods remain tricky.

Different technologies not only explore different scales of observations, but they do that through different physical methods, with possibly different responses to the same event. CRNS relies on the correlation of SM with the count of environmental neutrons, generated by cosmic rays and absorbed by hydrogen in water. While a standard conversion formula is widely used, it’s known to significantly deviate from experimental validation under extreme conditions of either dryness or wetness. For this reason, new formulas have been proposed and are in a phase of validation.

The SoMMet (Soil Moisture Metrology) project, funded by EURAMET (European Partnership on Metrology), was set up to develop metrological tools to enhance traceability and harmonization across different methods of SM observation. As part of the SoMMet project activities, various commercial CRNS probes were tested in SI-traceable reference neutron fields at participating national metrology institutes. The understanding of detector performance under laboratory conditions and the validation of Monte Carlo (MC) neutron transport modelling can be used to predict the detector response under real field conditions.

The development and validation of the specific MC model for the CRNS detector manufactured by Finapp has been recently published by the SoMMet Collaboration [1] and it introduces a new conversion formula. We will here review the SoMMet activities on characterization and MC model validation of the Finapp CRNS probe, performed in the reference neutron fields of Czech Metrology Institute (CMI) and Slovak Institute of Metrology (SMU) and consequent model verification at the Physikalisch-Technische Bundesanstalt (PTB), Germany.

As a first application to real-world conditions, we apply the SoMMet conversion formula to the datasets of two automated snow stations managed by the Office for Hydrology and Dams of the Civil Protection Agency of the Autonomous Province of Bolzano, Italy, equipped with Finapp CRNS sensors. The two sites (Pian dei Cavalli and Malga Fadner) are mountain sites at elevations above 2000 m, characterized by a very low soil bulk density and a very high water content, with presence of peatland in the footprint. The CRNS measurement was calibrated by the standard gravimetric campaign, but the standard conversion formula provides physically unrealistic results. The formula proposed by SoMMet is successfully applied.

[1] Z. Vykydal et al. (2025), Monte Carlo Simulation and Experimental Validation of the Finapp Model 3 Cosmic-Ray Neutron Sensor. Meas. Sci. Technol., in press, DOI:10.1088/1361-6501/ae2649

Aknowledgments: The project 21GRD08 SoMMet received funding from the European Partnership on Metrology, co-financed from the European Union’s Horizon Europe Research and Innovation Programme and by the Participating States.

How to cite: Gazzola, E., Vykydal, Z., Nadalet, R., Pernter, M., Dinale, R., Gianessi, S., and Biasuzzi, B.: The SoMMet characterization of a Finapp Cosmic-Ray Neutron Sensor and its first real-world application, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18160, https://doi.org/10.5194/egusphere-egu26-18160, 2026.

EGU26-18390 | ECS | Orals | GI4.7

Latitude Survey of Neutrons and Muons to Determine Cosmic Ray Neutron Sensing YieldFunction 

Lasse Hertle, Fraser Baird, Ulrich Schmidt, Bernd Heber, Michael Walter, Nora Krebs, Paul Schattan, Peter Dietrich, Steffen Zacharias, Solveig Landmark, Daniel Rasche, Marco Kossatz, Gary Womack, Steve Hamann, Enrico Gazzola, and Martin Schrön

Cosmic Ray Neutron Sensing (CRNS) is a ground based technique that utilises epithermal neutron measurements as a proxy for environmental hydrogen content. Similarly, to other ground based cosmic ray detectors (e.g. neutron monitors), CRNS detectors observe the solar cycle and space weather events. Typically, these effects must be corrected, but CRNS detectors have also been specifically used to observe space weather. The specific sensitivity of CRNS detectors to the primary spectrum and the relationship to other cosmic ray measurements is not fully understood. During the maximum of solar cycle 25 a latitude survey utilising a mini neutron monitor (MNM), two CRNS detectors of different design and a muon telescope was undertaken onboard the German Research Vessel Polarstern. The observations are used to derive differential response functions and yield functions for two neutron detectors. While the differential response, between neutron detectors is similar, it strongly deviates between muon and neutron detectors. The yield functions of CRNS and MNM are in good agreement with each other, indicating that CRNS detectors and MNM observe a comparable range of the primary cosmic ray spectrum.

How to cite: Hertle, L., Baird, F., Schmidt, U., Heber, B., Walter, M., Krebs, N., Schattan, P., Dietrich, P., Zacharias, S., Landmark, S., Rasche, D., Kossatz, M., Womack, G., Hamann, S., Gazzola, E., and Schrön, M.: Latitude Survey of Neutrons and Muons to Determine Cosmic Ray Neutron Sensing YieldFunction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18390, https://doi.org/10.5194/egusphere-egu26-18390, 2026.

EGU26-19012 | Orals | GI4.7

Exploring the inner structure of Esztramos Hill using cosmic rays 

Bence Rábóczki, Gergely Surányi, László Balázs, and Gergő Hamar

Cosmic-ray muography is a developing geophysical method that uses high energy cosmic muon particles to explore the inner structure of large objects, such as volcanoes, pyramids or mountains. Cosmic muons originate from upper atmosphere and have a known, steady, angle dependent flux on the surface. Muons are absorbed as they pass through matter, depending on the density of the material along their trajectories. By comparing the expected and the measured muon flux and using geoinformatic models of the observed area it is possible to calculate the density distribution inside these structures. Our research group at the HUN-REN Wigner Research Centre for Phyiscs has been conducting muographic measurements in the abandoned iron ore mine of Esztramos Hill (located in northeastern Hungary) for more than six years. Over the years we created muographic images of the hill from multiple drifts, resulting in a detailed understanding of its inner structure around the abandoned parts of the mine and the Rákóczi cave system, the main cave of which is part of the UNESCO World Heritage List. Based on a 3-D muographic inversion, our results were able to confirm the location of partially collapsed, inaccessible mined-out stopes and indicate the existence of a possible cave nearby, which was published in Scientific Reports last year.

How to cite: Rábóczki, B., Surányi, G., Balázs, L., and Hamar, G.: Exploring the inner structure of Esztramos Hill using cosmic rays, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19012, https://doi.org/10.5194/egusphere-egu26-19012, 2026.

EGU26-19089 | Orals | GI4.7

Results from a newly established long-term cosmogenic neutron observatory at kilometer scale with focus on soil water dynamics and distribution 

Sascha E. Oswald, Lena Scheiffele, Peter M. Grosse, Merlin Schiel, Maik Heistermann, and Till Francke

Cosmic-ray neutron sensing (CRNS) has shown its capability for estimating soil water content by providing spatially integrated measurements at an intermediate scale between invasive in-situ and satellite remote sensing observations. This constitutes a major advantage over point-scale sensors, which are often sparsely installed and are affected by small-scale heterogeneity, leading to uncertain absolute values. CRNS thus serves as an important link between local and larger scales and is increasingly used as a reference for remote sensing products and hydrological or land-surface models and other applications related to soil water balance. However, to fully close the scale gap observations are needed that reach the km scale.

Within the DFG-research Cosmic Sense and the European project SoMMet (21GRD08), a multiscale soil moisture monitoring was implemented by establishing a cluster of CRNS integrated with a range of complementary in-situ observations. This Potsdam Soil Moisture Observatory (PoSMO) was established in 2023 and features an accumulated CRNS footprint size of close to one km2 in total, constituting the largest long-term observation of epithermal cosmic-ray neutrons so far as well as the highest accumulated count rate of stationary CRNS worldwide. It comprises 16 stationary CRNS sensors located at an agricultural research site in the northeast of Germany, with some of the CRNS stations operated since end of 2019. They provide estimates of root-zone soil moisture at daily resolution, that is soil water content within the first decimeters of soil, but also co-located point-scale soil moisture measurements from shallow depth in 5 cm down to one meter. Intensive manual sampling campaigns of soil water content, bulk density, organic matter, and soil texture complement the dataset and enable robust CRNS calibration.

We discuss the PoSMO field set up, challenges associated with its design and the long-term monitoring operation. And we present the results of two years of harmonized soil water content time series from the different sensor types, including the CRNS cluster, shallow soil water content measurements, and soil water content profile data. Beyond the large area covered, CRNS and point sensors deliver also spatially resolved observations that will be shown as interpolated time-series of soil moisture maps for the inner part of the cluster. A sparser installation at the periphery and more singular sensors in the vicinity provide potential to even derive a soil moisture estimate for an area of up to 3.4 km2. Also, the potential benefit of accompanying physical measurements of the neutron spectrum (via Bonner spheres), muon measurements with a scintillator-based CRNS or roving CRNS may be discussed as well as the link to the Brandenburg state CRNS network.

How to cite: Oswald, S. E., Scheiffele, L., Grosse, P. M., Schiel, M., Heistermann, M., and Francke, T.: Results from a newly established long-term cosmogenic neutron observatory at kilometer scale with focus on soil water dynamics and distribution, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19089, https://doi.org/10.5194/egusphere-egu26-19089, 2026.

EGU26-19701 | ECS | Orals | GI4.7

Environmental Neutron Spectrometry: Continuous outdoor measurement with the PTB Bonner sphere spectrometer NEMUS-UMW 

Jonas Marach, Markus Köhli, Jannis Weimar, Peter Grosse, Marcel Reginatto, and Miroslav Zboril

After three years, the European research project SoMMet (Soil Moisture Metrology) has come to an end. One of PTB’s (Physikalisch-Technische Bundesanstalt) tasks within this collaboration with 17 other institutes was to develop the Bonner sphere spectrometer (BSS) system NEMUS-UMW, capable of performing continuous, automated neutron spectrometry under outdoor conditions. PTB now plans to continue these activities by identifying new scientifically interesting sites for such measurements.

The BSS NEMUS-UMW uses 11 proportional counters to detect the neutron component of secondary cosmic radiation. By varying the sizes (3" to 10" in diameter) of the polyethylene moderating spheres surrounding the counters, and by using copper or lead shells in the larger spheres, the system covers an energy range from 10⁻⁹ MeV to 10³ MeV. Using the known response functions of the individual spheres, the neutron energy spectrum can be unfolded. The system was calibrated in the PTB neutron reference fields and is therefore capable of determining outdoor neutron spectra and radiation levels in absolute units of neutron fluence rate.

During SoMMet, the BSS NEMUS-UMW was deployed at the test field site ATB Marquardt (Potsdam, Germany). In collaboration with the University of Potsdam and Heidelberg University, surrounding field and soil parameters were monitored, and the measured neutron-spectrum time series was used to benchmark URANOS-based neutron simulations.

In January 2026, the BSS NEMUS-UMW was installed on the PTB premises in Braunschweig (Germany), where it has also been used to study the impact of heavy snowfall on neutron radiation in early 2026.

This presentation introduces the BSS NEMUS-UMW setup and data analysis, including corrections for environmental influences, and compares measurement results with simulations.

How to cite: Marach, J., Köhli, M., Weimar, J., Grosse, P., Reginatto, M., and Zboril, M.: Environmental Neutron Spectrometry: Continuous outdoor measurement with the PTB Bonner sphere spectrometer NEMUS-UMW, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19701, https://doi.org/10.5194/egusphere-egu26-19701, 2026.

EGU26-20428 | Posters on site | GI4.7

COSMOS-UK incoming neutron intensity correction case study for soil moisture monitoring using cosmic-ray neutron sensors 

Jonathan Evans, Magdalena Szczykulska, and Tim Howson and the COSMOS-UK Team

Cosmic-ray neutron sensors (CRNSs) provide state-of-the-art soil moisture measurements at a field scale. This sensing technique utilises cosmic-ray neutrons which need to be corrected for any temporal changes due to the external factors other than soil moisture. These typically include corrections for changes in humidity, pressure and the incoming flux of neutrons. The last correction is strongly linked with the changes in the solar activity and typically uses standardized neutron monitors (NMs), which are in operation around the world, as the reference signal. Different approaches have emerged for calculating the correction parameter, often referred to as ‘tau’, which accounts for location differences between the CRNS and NM stations. This work is a case study of the published incoming neutron flux correction parameters (taus) applied to the UK COsmic-ray Soil Moisture Observing System (COSMOS-UK) network. We investigate the impact of the different approaches on the resulting soil moisture and compare them against a correction parameter derived using the local CRNS data (gamma), and also against the available point sensor soil moisture measurements. We discuss the potential causes of discrepancies between the published (tau-based) methods and our insitu (gamma-based) method, especially in the context of soil moisture trends visible at some COSMOS-UK sites when using the tau-based methods.

How to cite: Evans, J., Szczykulska, M., and Howson, T. and the COSMOS-UK Team: COSMOS-UK incoming neutron intensity correction case study for soil moisture monitoring using cosmic-ray neutron sensors, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20428, https://doi.org/10.5194/egusphere-egu26-20428, 2026.

EGU26-20506 | ECS | Posters on site | GI4.7

Observations of GLE 77 from the Ground, On Aircraft and Balloons 

Fraser Baird, Ben Clewer, Chris Davis, Keith Ryden, Clive Dyer, and Fan Lei

Cosmic rays generate an ever-present radiation field in Earth’s atmosphere, right down to the ground. On rare occasions, high energy particles accelerated at the Sun can increase this radiation field, in events known as Ground Level Enhancements (GLEs). November 11th 2025 saw the strongest GLE in nearly 25 years: GLE 77. The event resulted in the count rate of some sea level neutron monitors exceeding 100% of the pre-event mean. In this contribution, we present a comprehensive set of observations of the event made from the UK and the Netherlands. At ground level, we present data from the Compact Neutron Monitors in Guildford, in the south of the England, and Shetland, off the north coast of Scotland. Dose rate measurements are presented from SAIRA instruments onboard two trans-Atlantic flights during the event. In addition, the data from SAIRA instruments onboard weather balloons, launched from Shetland, Cornwall, and the Netherlands, are presented. Finally, modelling results derived from the MAIRE-S system will be shown briefly.

How to cite: Baird, F., Clewer, B., Davis, C., Ryden, K., Dyer, C., and Lei, F.: Observations of GLE 77 from the Ground, On Aircraft and Balloons, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20506, https://doi.org/10.5194/egusphere-egu26-20506, 2026.

EGU26-20716 | Posters on site | GI4.7

Neptoon: An open-source and extensible software tool for data processing of cosmic-ray neutron sensors  

Martin Schrön, Daniel Power, Markus Köhli, Rafael Rosolem, Till Francke, Louis Trinkle, Fredo Erxleben, and Steffen Zacharias

The highly interdisciplinary method of Cosmic Ray Neutron Sensing (CRNS) has emerged as a key technology for monitoring root-zone soil moisture at the hectare scale. The technique bridges the spatial gap between traditional point-scale measurements and coarser remote sensing products. While CRNS is widely used in agriculture and weather services, processing of its data requires advanced knowledge about cosmic-ray physics. With the increasing adoption of CRNS across research infrastructures and observatories world-wide, standardised, flexible, and easy-to-use processing tools are essential for supporting data integration within these networks. Here we present neptoon, an open-source Python tool for neutron data processing that addresses these highly interdisciplinary challenges. It implements a modular, expandable framework to support both operational deployment of CRNS, as well as methodological innovation. Building from previous CRNS processing tools, we will present the overall architecture of neptoon and how it implements established processing methodologies while maintaining extensibility for emerging approaches. Through an intuitive configuration system and graphical user interface, neptoon streamlines data processing workflows and ensures reproducibility across research sites. As our understanding of the sensor signal continues to improve, the ability for research infrastructures to quickly implement the latest advancements becomes ever more important. We will demonstrate how neptoon facilitates rapid deployment of these latest processing methodologies, supports cross-site harmonisation, whilst also enabling robust testing of experimental correction methods. Through its support of multiple stakeholders, from researchers to sensor owners, the latest advancements can be pushed quickly back to the broader community. By providing a standardised yet flexible processing framework, neptoon aims to accelerate the integration of CRNS measurements into critical zone research and enhance our understanding of soil moisture dynamics across scales.

How to cite: Schrön, M., Power, D., Köhli, M., Rosolem, R., Francke, T., Trinkle, L., Erxleben, F., and Zacharias, S.: Neptoon: An open-source and extensible software tool for data processing of cosmic-ray neutron sensors , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20716, https://doi.org/10.5194/egusphere-egu26-20716, 2026.

EGU26-21790 | ECS | Orals | GI4.7

Linking field-scale soil water regimes with vegetation response using CRNS and soil hydrophysical thresholds: a case study in Ireland 

Konstantin Shishkin, Owen Fenton, Paul Murphy, Klara Finkele, and Tamara Hochstrasser

Reliable assessment of soil water regime at the field scale is essential for understanding plant–soil interactions in managed grassland systems, yet remains challenging due to strong spatial heterogeneity and scale mismatches between soil moisture observations and vegetation response. Point-scale sensors provide detailed local measurements but often fail to represent field-scale conditions, while integrative approaches require independent validation to ensure their relevance for agrosystem functioning.

This study presents an integrated framework combining Cosmic-Ray Neutron Sensing (CRNS) with soil hydrophysical characterisation based on Soil Water Retention Curves (SWRC) to assess soil water regime dynamics and their relationship with vegetation response. CRNS-derived volumetric water content was interpreted relative to physically meaningful hydrophysical thresholds obtained from SWRC analysis, enabling continuous classification of soil moisture conditions across wet, optimal, and water-limited regimes.

Vegetation data were used as an independent indicator of soil water status to evaluate the consistency of CRNS–SWRC-derived regimes with observable plant responses. Field-scale grass growth dynamics were compared against classified soil moisture regimes to assess whether transitions in soil water availability were reflected in changes in vegetation productivity. This comparison allowed the identification of periods where vegetation response deviated from expected soil moisture conditions, highlighting potential anomalies related to root-zone decoupling, management interventions, or sub-footprint soil heterogeneity.

The results demonstrate that the combined CRNS–SWRC approach captures seasonal and event-scale variability in soil water regimes that correspond with observed grass growth patterns. At the same time, mismatches between soil moisture regimes and vegetation response provide valuable diagnostic information, enabling the detection of anomalous conditions not evident from soil moisture data alone.

The proposed framework extends beyond soil moisture monitoring by linking integrative hydrological measurements with biological response, offering a robust tool for field-scale assessment of soil–plant water interactions. This approach supports improved interpretation of soil water dynamics in heterogeneous agricultural landscapes and provides a foundation for anomaly detection and decision support in grassland management.

How to cite: Shishkin, K., Fenton, O., Murphy, P., Finkele, K., and Hochstrasser, T.: Linking field-scale soil water regimes with vegetation response using CRNS and soil hydrophysical thresholds: a case study in Ireland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21790, https://doi.org/10.5194/egusphere-egu26-21790, 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.

EGU26-75 | 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.

EGU26-1565 | Orals | AS3.11

Evaluating dust storms modeled at kilometer-scale resolution in the ECOMIP initiative 

Martina Klose, Andreas Baer, Rumeng Li, Noel M. Chawang, Natalie Ratcliffe, and Sebastian Vergara Palacio

Advanced kilometer-scale resolution modeling offers unprecedented detail of atmospheric processes and properties, including of mineral dust. At kilometer-scale model resolutions, deep moist convective processes do not have to be parameterized any more, but can be represented explicitly at the grid resolution. These processes are very effective in transporting heat, moisture, and energy within the atmosphere and therefore have strong impacts on weather phenomena, such as wind storms. Mineral dust emission is a threshold process that depends non-linearly upon surface wind intensity, which means that the accuracy at which models represent surface winds, together with land-surface properties, is key to estimating dust emissions. A spectacular and intense type of dust storm, i.e. haboob dust storms, is caused by the cold pool outflow of moist convection. We therefore expect that the explicit representation of moist convection in kilometer-scale simulations is particularly beneficial for dust modeling. Determining whether kilometer-scale models can meet this expectation, demands in-depth evaluation against observations. This evaluation is now enabled through novel satellite missions, such as the Earth Cloud Aerosol and Radiation Explorer (EarthCARE). Here we present results of kilometer-scale simulations conducted with two models, ICON-ART and ICON-HAM-lite, both including an interactive dust representation. We investigate, for example, evaporative cooling and vertical velocities associated with moist convection as drivers of dust emission. We compare our results against observations from EarthCARE and ORCESTRA (Organized Convection and EarthCARE Studies over the Tropical Atlantic), and against results from other models in the framework of the EarthCARE-ORCESTRA Model Intercomparison Project (ECOMIP). Our results show fascinating detail of mineral dust processes, enabling novel insights into the mineral dust cycle, for example, a globally consistent characterization of haboob properties and impacts.

How to cite: Klose, M., Baer, A., Li, R., Chawang, N. M., Ratcliffe, N., and Vergara Palacio, S.: Evaluating dust storms modeled at kilometer-scale resolution in the ECOMIP initiative, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1565, https://doi.org/10.5194/egusphere-egu26-1565, 2026.

EGU26-1791 | Posters on site | AS3.11

Assessing aerosol impacts on EarthCARE radiative closure using spectral radiation observations 

Stelios Kazadzis and the RACE ECV Thessaloniki Campaign Team

Satellite-based radiation retrievals are essential for quantifying the Earth’s radiative energy budget and for climate-related studies. The EarthCARE (EC) mission aims to improve our understanding of how aerosols and clouds modify radiative fluxes by providing collocated radiation observations and products based on a three-dimensional representation of atmospheric constituents. The evaluation of these products is therefore crucial for accurately estimating aerosol and cloud radiative effects.

In this study, we assess EC radiation products and their associated aerosol and cloud inputs by conducting radiative closure experiments using ground-based spectral radiation and aerosol measurements acquired during the RACE-ECV (Radiation Closure Experiments for EarthCARE Validation) field campaign.

The RACE-ECV campaign was coordinated by PMOD/WRC — the world reference institute for solar measurements and aerosol optical depth as designated by the World Meteorological Organization (WMO) — with the participation of multiple institutions. Its primary objective was the validation of EarthCARE products through high-accuracy measurements of solar radiation and aerosols. The campaign was conducted in spring 2025 (April 22–May 22) at three coordinated sites in Thessaloniki area, aligned with EC satellite overpasses. High-accuracy sun photometers were deployed in synergy with other ground-based remote-sensing instruments, comprehensive observations of aerosols, clouds, and surface solar spectral radiation.

The radiative closure at the surface was assessed through an intercomparison between measured broadband and spectral solar fluxes and radiative transfer (RT) simulations driven by both ground-based and EC atmospheric inputs. In particular, EarthCARE reconstructed three-dimensional atmospheric fields were used as input to the 3D/1D MYSTIC code (Mayer, 2009) to assess the accuracy of surface radiation products, while simultaneously quantifying the contribution of individual input parameters (focusing on aerosols) to the observed discrepancies. In addition, simulated fluxes at the top of the atmosphere (TOA) were intercompared with EC Broadband Radiometer (BBR) observations.

This study provides insights into the use of EarthCARE observations for improving our understanding of the role of aerosols and clouds in modifying the Earth’s radiative energy fluxes. 

 References:

Emde, C., et al.: The libRadtran software package for radiative transfer calculations (version 2.0.1), Geosci. Model Dev., 9, 1647–1672, https://doi.org/10.5194/gmd-9-1647-2016, 2016

Mayer, B. (2009) Radiative transfer in the cloudy atmosphere, in: EPJ Web of Conferences, 75–99.

Mayer B. and Kylling A., Technical note: The libRadtran software package for radiative transfer calculations - description and examples of use. Atmos. Chem. Phys., 5: 1855-1877, 2005

Acknowledgements:

The authors acknowledge the project RACE-ECV, (SBFI-633.4-2021-2024/PMOD - EarthCARE 202/2) supported by SBFI, the the Horizon Europe European Research Council (grant no. 101137680, Cloud–aERosol inTeractions & their impActs IN The earth sYstem, CERTAINTY) and the Obs3RvE (Optimising 3D RT EarthCARE product using geostationary observations and AI) project, funded from the European Space Agency under Contract No. 4000147848/25/I/AG.

How to cite: Kazadzis, S. and the RACE ECV Thessaloniki Campaign Team: Assessing aerosol impacts on EarthCARE radiative closure using spectral radiation observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1791, https://doi.org/10.5194/egusphere-egu26-1791, 2026.

EGU26-3759 | ECS | Posters on site | AS3.11

Validation of the EarthCARE ACM_RT product using surface solar irradiance measurements from BSRN stations and modeled values from CAMS. 

Yannis Gschwind, Kyriakoula Papachristopoulou, and Stelios Kazadzis

The EarthCARE (ECA) satellite is currently in its second year in orbit, collecting new data every
day that could play a crucial role in advancing climate science. However, due to the advanced
technologies and retrieval approaches used in EarthCARE, the credibility of each instrument and
of their synergetic products must be verified. Significant effort has been devoted to this topic
both currently and in the past. Nevertheless, a substantial amount of publicly available data
that could improve validation has not yet been used. In this study, we use the ground-based
radiation measurements from the Baseline Surface Radiation Network (BSRN) to validate
1D surface solar radiation estimates from the EarthCARE ACM_RT product. Cloud effects are
analyzed separately using the cloud modification factor approach. Values from BSRN stations
are used if the station has less than 50 km distance to the satellite ground track. In addition,
an intercomparison with Copernicus Atmospheric Monitoring Service (CAMS) satellite based
surface solar radiation estimations has been performed. For the comparison with CAMS,
ECA values are averaged over time to obtain collocated grid cells. Due to limited gridded data
availability of the CAMS radiation service, this comparison is restricted to September-December
2024.

The ECA surface solar irradiance exhibits a Mean Bias Error (MBE) of −10.4 Wm-2 and a
Root Mean Square Error (RMSE) of 191.7 Wm-2 against ground based (BSRN) measurements.
Relative to CAMS, ECA surface solar irradiance exhibits a MBE of −23.3 Wm-2 and a RMSE
of 103.3 Wm-2. While some parts of South America, Northern Africa and Western Asia tend to
have higher EarthCARE irradiance, most of the available regions show higher CAMS irradiance.
This is especially the case in Oceania, middle part of Africa and Europe. Approximately 69%
of the difference between EarthCARE and CAMS can be contributed to differences in cloud
estimation, while 31% can be contributed to differences in clear-sky irradiance.

Future data releases from BSRN and CAMS are expected to enable a more robust assessment.
This analysis offers valuable insights relevant to the solar energy community.

Acknowledgements:

The authors acknowledge the project RACE-ECV (SBFI-633.4-2021-2024/PMOD - EarthCARE 202/2), supported by SBFI, the project Observe: Optimising 3D RT Earthcare product using geostationary observations and AI,  ESA Contract No. 4000147848/25/I/AG and the CERTAINTY (Cloud aERosol inTeractions & their impActs IN The earth sYstem) project funded from the Horizon Europe programme under Grant Agreement No 101137680

How to cite: Gschwind, Y., Papachristopoulou, K., and Kazadzis, S.: Validation of the EarthCARE ACM_RT product using surface solar irradiance measurements from BSRN stations and modeled values from CAMS., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3759, https://doi.org/10.5194/egusphere-egu26-3759, 2026.

EGU26-8723 | ECS | Posters on site | AS3.11

Comparison of spaceborne retrieved vertical velocity and latent heating profiles using the EarthCARE–GPM coincidence dataset 

Shunsuke Aoki, Takuji Kubota, and Shoichi Shige

Latent heat (LH) released by precipitating cloud systems is a primary driver of vertical air motion (Vair) within clouds and plays a crucial role in transporting energy from the Earth’s surface to the atmosphere. In the Tropical Rainfall Measuring Mission (TRMM) and its successor, the Global Precipitation Measurement (GPM) mission, LH profiles associated with condensation and evaporation processes have been estimated using precipitation observations from spaceborne Ku-band radars. In contrast, Doppler radar measurements from the Cloud Profiling Radar (CPR) onboard the Earth Cloud Aerosol and Radiation Explorer (EarthCARE) enable global observations of vertical motions within clouds. Vair is retrieved by subtracting estimated hydrometeor fall speeds, inferred from radar reflectivity together with collocated atmospheric lidar and multispectral imager observations, from the measured Doppler velocities. With these complementary observations, we investigated how consistent the GPM-derived LH profiles are with the EarthCARE-derived Vair profiles.

We have developed the EarthCARE–GPM coincidence dataset, which compiles cases in which the ground tracks of the two satellites intersect. The dataset extracts data from coincident segments while preserving the original structure of all Level-2 standard products from the four EarthCARE sensors, namely the cloud radar, lidar, imager, and broad-band radiometer, as well as the two GPM sensors, namely the precipitation radar and microwave radiometer. Using this dataset, we directly compared Vair derived from EarthCARE Doppler measurements, including both the JAXA’s standard product and an alternative retrieval based on the method introduced in Aoki et al. (2026), with LH profiles from the GPM Spectral Latent Heating product. Analyses classified by precipitation type reveal physically consistent relationships. Convective precipitation exhibits deep tropospheric heating accompanied by upward motions throughout the column. In contrast, stratiform precipitation shows top-heavy heating above the melting layer with corresponding upper-level ascent, while both LH and Vair are close to zero in the lower troposphere. Nevertheless, substantial uncertainties remain in the estimation of each product, and continued intercomparison between these complementary observations remains important for assessing and improving the reliability of both estimates.

How to cite: Aoki, S., Kubota, T., and Shige, S.: Comparison of spaceborne retrieved vertical velocity and latent heating profiles using the EarthCARE–GPM coincidence dataset, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8723, https://doi.org/10.5194/egusphere-egu26-8723, 2026.

EGU26-10155 | Orals | AS3.11

Advancing Ocean and Land Surface Remote Sensing with EarthCARE’s lidar ATLID 

Gerd-Jan van Zadelhoff, John Smith, Brian Collister, Dave Donovan, Diko Hemminga, Jonathan Hair, Chris Hostetler, and Taylor Shingler

The ESA-JAXA EarthCARE mission delivers cutting‑edge measurements of clouds, aerosols, and Earth’s radiation budget, quantifying the coupled interactions among the three. A key instrument on the mission is the high‑spectral‑resolution lidar (ATLID), which produces data useful beyond its primary role in atmospheric science. Although developed for atmospheric observations, ATLID’s ability to quantify the near-surface ocean backscatter also supports ocean‑optical applications, including examining how subsurface lidar signal attenuation is influenced by optical constituents such as phytoplankton and colored dissolved organic matter.

The co‑polar Mie surface return from ATLID provides estimates of aerosol and cloud optical depth, which are essential for calibrating the near-surface ocean Rayleigh signal. Once corrected for atmospheric attenuation, the isolated Rayleigh component can be used to infer chlorophyll concentrations using established bio-optical models. The surface depolarization ratio from ATLID also enables reliable discrimination between ocean and sea ice, ensuring chlorophyll retrievals are limited to open-water areas. The methodology’s validation includes using NASA HSRL2 data from the NightBLUE campaign to corroborate ocean subsurface retrievals.

The global performance of ATLID-derived chlorophyll retrievals is validated through comparisons with established satellite data from PACE-OCI, Aqua-MODIS and Sentinel-3 OLCI, as well as reanalysis products from the Copernicus Marine Environment Monitoring Service (CMEMS). Initial findings show strong agreement, with ATLID successfully capturing large-scale chlorophyll gradients, particularly in open-ocean areas. ATLID’s ability to operate in high latitudes and night-time conditions, where passive sensors face limitations, represents an important step forward. These capabilities show promise in extending the temporal and spatial coverage of ocean-color data. The retrieved chlorophyll concentrations may be used to help refine estimates of ocean albedo within EarthCARE’s Level 2 radiative‑closure studies.

Additionally, over land ATLID surface depolarization ratios correlates well with the Normalized Difference Vegetation Index (NDVI) and, over desert surfaces, also shows a relationship with the TROPOMI Lambertian Equivalent Reflectance (LER). This demonstrates ATLID’s ability to characterize surface-atmosphere interactions and reinforces its relevance across both ocean and land domains.

In summary, EarthCARE ATLID’s surface return, corrected for aerosol attenuation using the co-polar Mie surface returns, introduces a novel and unique method for global chlorophyll retrievals. This first demonstration showcases how atmospheric lidar can complement existing remote sensing products like MODIS, OLCI, and CMEMS, while offering valuable contributions to both ocean and land classification, such as desert albedo and NDVI analysis.

How to cite: van Zadelhoff, G.-J., Smith, J., Collister, B., Donovan, D., Hemminga, D., Hair, J., Hostetler, C., and Shingler, T.: Advancing Ocean and Land Surface Remote Sensing with EarthCARE’s lidar ATLID, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10155, https://doi.org/10.5194/egusphere-egu26-10155, 2026.

EGU26-10702 | ECS | Orals | AS3.11

Combining the German national radar network with EarthCARE's Cloud Profiling Radar 

Christian Stefan Heske, Florian Ewald, and Silke Groß

The understanding of microphysical properties and processes in clouds plays a substantial role in the improvement of existing numerical weather models and forecasting. To gain access to these quantities deep within clouds, microphysical retrievals based on radar measurements are indispensable tools. Single-wavelength radar measurements, however, are not enough to properly constrain the microphysical properties of hydrometeors like size and shape alone and therefore need to be paired with other measurement techniques like multi-wavelength or polarimetric quantities. While polarimetric quantities are mainly useful from an oblique perspective, multi-wavelength or Doppler fall-speed observations are best made vertically. 

To tackle this observational dilemma, we combine data provided by the vertically pointing W-band Cloud Profiling Radar (CPR) carried on EarthCARE with data generated by the national German radar network operated by the Deutscher Wetterdienst (DWD) which consists of 17 polarization Doppler weather radars in the C-band covering whole Germany together. Vertical profiles from operational scans in range of EarthCare's overpasses are extracted at the position of the footprint of CPR following the recently developed Beam-aware Columnar Vertical Profile (BA-CVP) method. This measurement geometry grants the opportunity to combine multi-wavelength radar observations with Doppler fall-speed measurements and side-looking polarimetry for the possibility of constraining existing ambiguities concerning the microphysical properties of ice hydrometeors. 

The findings of this study in form of more accurate information about ice hydrometeors based on polarimetric multi-frequency radar measurements can ultimately be used to improve existing numerical weather models with regards to ice growth processes and their representation within the models. Naturally, similar studies can be done for any other operational radar network overflown by EarthCARE by adapting the BA-CVP method, opening the door for quasi-global dual-wavelength radar observations on an operational scale.

How to cite: Heske, C. S., Ewald, F., and Groß, S.: Combining the German national radar network with EarthCARE's Cloud Profiling Radar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10702, https://doi.org/10.5194/egusphere-egu26-10702, 2026.

EGU26-12433 | Orals | AS3.11

EarthCARE observes the life cycle of a stratospheric smoke plume  

Holger Baars, Moritz Haarig, Leonard König, Dave Donovan, Albert Ansmann, Sergey Khaykin, Romain Ceolato, Jason Cole, Benedikt Gast, Athena Augusta Floutsi, Valentin Jakob Heckmann, Robin Hogan, Annabel Chantry, Fabien Marnas, Gerd-Jan Zadelhoff van, and Ulla Wandinger

At the end of May 2025, extremely strong wildfires in Canada produced several pyrocumulonimbus clouds which lifted wildfire smoke particles up to the lower stratosphere (> 10 km height). A dense stratospheric smoke plume developed which reached stratospheric aerosol optical depths up to 3.2 which is comparable with a moderate volcanic eruption. EarthCARE’s lidar ATLID captured this event and enabled us to study stratospheric smoke shortly after emission and to track a single smoke plume on its transport way towards Europe.
The spaceborne lidar allowed to precisely study the maximum plume height and revealed a lofting of the smoke plume top height from 13.6 km above Canada to 17.4 km above Europe and a further slight ascent during the transport towards Asia. The self-lofting of dense smoke plumes can be explained by the absorption of solar radiation which heats the ambient air and creates buoyancy. The self-lofting is strongest for optically thick smoke plumes close to the source region and gets weaker when the plume is horizontally more spread and thus optically thinner.
ATLID detected an enhanced depolarization ratio of 0.26±0.02 which indicates non-spherical smoke particles in the stratosphere. This finding is in line with previous observations of stratospheric smoke layers, but clearly demonstrates a difference to tropospheric observations of Canadian smoke in Europe, which are characterized by a low depolarization ratio and hence a spherical shape (Haarig et al., 2018).
The novel high-spectral-resolution lidar (HSRL) capability of ATLID allowed us for the first time to study the evolution of the lidar ratio of a stratospheric smoke layer during long-range transport. Higher values around 70 sr were observed shortly after emission, which decreased during the first days of transport to values of 49±7 sr.
As another highlight, EarthCARE observed a significant downmixing of stratospheric smoke at a strong tropopause fold over the Mediterranean and North Africa (Haarig et al., 2025). These observations directly show a pathway of removal of the stratospheric smoke and closes the life cycle from injection to removal. Additionally, the synergistic EarthCARE observations will be used to estimate the radiative impact of this strong stratospheric smoke event.

References

Haarig, M., et al. (2018), Depolarization and lidar ratios at 355, 532, and 1064 nm and microphysical properties of aged tropospheric and stratospheric Canadian wildfire smoke. Atmospheric Chemistry and Physics, 18 (16), 11847–11861.

Haarig, M. et al. The life cycle of a stratospheric smoke plume as seen from EarthCARE - tracking a plume from Canada to Europe. ESS Open Archive. October 22, 2025.

How to cite: Baars, H., Haarig, M., König, L., Donovan, D., Ansmann, A., Khaykin, S., Ceolato, R., Cole, J., Gast, B., Floutsi, A. A., Heckmann, V. J., Hogan, R., Chantry, A., Marnas, F., Zadelhoff van, G.-J., and Wandinger, U.: EarthCARE observes the life cycle of a stratospheric smoke plume , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12433, https://doi.org/10.5194/egusphere-egu26-12433, 2026.

EGU26-13319 | ECS | Posters on site | AS3.11

Validation of EarthCARE-Derived Planetary Boundary Layer Height Using the E-Profile Ceilometer Network and Radiosondes  

Onel Rodríguez-Navarro, Jorge Muñiz-Rosado, Alexander Haefele, Eric Sauvageat, Arlett Díaz-Zurita, Víctor Manuel Naval-Hernández, Alberto Cazorla, Daniel Pérez-Ramírez, Lucas Alados-Arboledas, and Francisco Navas-Guzmán

The Earth Clouds, Aerosol and Radiation Explorer (EarthCARE), launched in May 2024 as a joint ESA–JAXA mission, provides vertically resolved observations of aerosols and clouds with unprecedented sensitivity from space. In this study, we exploit measurements from the Atmospheric Lidar (ATLID), a high-spectral-resolution lidar operating at 355 nm, whose enhanced signal-to-noise ratio and capability to separate molecular and particulate backscatter enable detailed characterization of the lower troposphere (Wehr et al., 2023). These features make ATLID particularly suitable for deriving the planetary boundary layer height (PBLH) at the global scale.

The PBL is the atmospheric layer most strongly influenced by surface forcing through turbulent exchanges of heat, moisture and momentum. Accurate estimates of PBLH are therefore essential for weather forecasting, climate modelling and air quality studies. Previous spaceborne lidar missions, notably CALIPSO, demonstrated the feasibility of PBLH retrievals from aerosol backscatter profiles, although with limitations related to signal attenuation, cloud contamination and retrieval robustness (McGrath-Spangler and Denning, 2012). EarthCARE’s ATLID offers enhanced capabilities to address these challenges.

We validate ATLID-derived PBLH using independent ground-based observations from the E-Profile network, comprising over 400 ceilometers across Europe, along with collocated radiosonde measurements from the University of Wyoming Upper Air Soundings database. A continental-scale reference dataset was generated by applying the STRATfinder algorithm to ceilometer aerosol backscatter profiles. Planetary boundary layer heights from radiosondes were independently estimated using several thermodynamic and dynamical approaches, including the bulk Richardson number, the parcel method, and gradient-based criteria applied to temperature and humidity profiles. Only radiosonde launches collocated with E-Profile stations were considered, ensuring spatial consistency among the reference datasets. The analysis includes 580 collocated cases, defined as EarthCARE overpasses within 20 km of a ground-based station, from which 25 correspond to radiosonde observation, covering the period from August 2024 to August 2025.

Two complementary approaches were assessed to retrieve PBLH from ATLID Level-2 BA baseline products. The first approach used the operational A-ALD product, which includes PBLH as a retrieved variable. The product showed limitations, with misidentification of cloud layers as the PBL and a lack of retrievals under favourable conditions. These results underline current shortcomings of A-ALD for PBL detection, while indicating potential for future algorithm improvements.

The second approach applied combined variance–gradient methods to attenuated backscatter profiles from the A-EBD product, supported by cloud screening using the A-FM product. This strategy allowed more robust and physically consistent PBLH estimates. The comparison with ground-based ceilometer references resulted in a standard deviation of 343 m and a mean bias of 101 m. The nearly symmetric uncertainty distribution highlights the reliability of this approach. Radiosonde-based results showed a clear dependence on the retrieval method, with the best performance obtained for gradient-based approaches, although their statistical representativeness is limited by the small number of available cases.

These findings highlight the capability of EarthCARE’s ATLID to capture the PBL from space for climatological and modeling applications. The validation also emphasizes the importance of networks such as E-Profile, which provide the necessary reference data to evaluate satellite-derived boundary layer products on a continental scale.

How to cite: Rodríguez-Navarro, O., Muñiz-Rosado, J., Haefele, A., Sauvageat, E., Díaz-Zurita, A., Naval-Hernández, V. M., Cazorla, A., Pérez-Ramírez, D., Alados-Arboledas, L., and Navas-Guzmán, F.: Validation of EarthCARE-Derived Planetary Boundary Layer Height Using the E-Profile Ceilometer Network and Radiosondes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13319, https://doi.org/10.5194/egusphere-egu26-13319, 2026.

EGU26-14141 | Orals | AS3.11

Global Retrievals of Cloud Condensation Nuclei and Aerosol Absorption based on the first year of EarthCARE ATLID observations 

Jens Redemann, Lan Gao, Bradley Lamkin, Philip Stier, Dave Donovan, Gerd-Jan van Zadelhoff, Silke Gross, and Martin Wirth

Studies of aerosol-cloud interactions and estimates of the effective aerosol radiative forcing (ERF) of climate depend crucially on the vertical distribution of aerosol microphysical and radiative properties, but few reliable observations of such properties exist on a global scale. The 2024 launch of the EarthCARE mission provides new observations of aerosol extinction from the ATMospheric LIDar (ATLID) system. These observations are proving to be superior to past satellite-based lidar observations of aerosol extinction in accuracy because of the use of the high-spectral resolution lidar (HSRL) technique. These high-accuracy lidar observations can be used as input to machine-learning (ML) models to estimate cloud condensation nuclei (CCN at 0.4% supersaturation) and aerosol absorption (ABS at 532nm).

We present novel ML-based CCN and ABS retrievals using the first full year of ATLID observations (September 2024 to August 2025) of aerosol backscatter, extinction, and depolarization as predictors. These higher-level aerosol properties are compared to retrievals of the same quantities derived from airborne HSRL observations by the WALES system (derived from WAter vapor Lidar Experiment in Space) during the ORCESTRA (ORganized Convection and EarthCARE STudies over the Tropical Atlantic) PERCUSION (Persistent EarthCARE Underflight Studies of the ITCZ and Organized Convection) campaign in the summer of 2024. We provide validation results of the ML-based CCN and ABS retrievals against ground-based in situ observations, which indicate relative errors less than 30% for all but the cleanest aerosol loading conditions. Based on the first year of ATLID observations, we present global maps of ML-derived CCN and ABS and suggestions for improvements in the ATLID observations. Finally, we discuss opportunities to study aerosol-cloud-climate interactions facilitated by these new retrievals and climatologies.

How to cite: Redemann, J., Gao, L., Lamkin, B., Stier, P., Donovan, D., van Zadelhoff, G.-J., Gross, S., and Wirth, M.: Global Retrievals of Cloud Condensation Nuclei and Aerosol Absorption based on the first year of EarthCARE ATLID observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14141, https://doi.org/10.5194/egusphere-egu26-14141, 2026.

EGU26-16100 | ECS | Orals | AS3.11

Evaluation of Doppler Velocity in a GSRM Using the EarthCARE Satellite with Implications for Improving Model Cloud Microphysics 

Shuhei Matsugishi, Yuhi Nakamura, Tatusya Seiki, Woosub Roh, Kentaroh Suzuki, and Masaki Satoh

Conventional climate and numerical weather prediction models have long relied on empirical parameterizations of hydrometeor fall speeds, which have not been comprehensively validated on the global scale due to a lack of their global observations. Nevertheless, fall-speed parameters strongly influence model performance and are often subject to tuning. For example, Takasuka et al. (2024) showed that modifying the fall speeds of snow and rain improves the representation of both climate-scale statistics and intraseasonal variability. However, such tuning is not directly constrained by observations; instead, parameter values are selected to best reproduce large-scale climate fields and disturbances.

Notable in this regard is the recent emergence of the EarthCARE satellite, launched in late May of 2024, which provides the first-ever global observations of the vertical motion of hydrometeors from space. In this study, we compare representative fall-speed parameter settings in the Nonhydrostatic Icosahedral Atmospheric Model (NICAM) against EarthCARE observations. We use a single-moment cloud microphysics scheme (Tomita, 2008; Roh and Satoh, 2014) with two configurations. One employs the tuned fall-speed parameters proposed by Takasuka et al. (2024), while the other follows the original parameterization used in Kodama et al. (2021). The Takasuka et al. (2024) configuration prescribes slower fall speeds for both snow and rain than the Kodama et al. (2021) setting. To enable a consistent comparison with EarthCARE, EarthCARE-like observables are generated using the Joint Simulator for Satellite Sensors (Hashino et al., 2013) and evaluated against satellite measurements.

The results show that the Takasuka et al. (2024) configuration produces snow and rainfall fall speeds that are closer to EarthCARE observations than those obtained with the Kodama et al. (2021) setting, although it tends to overestimate radar reflectivity. In addition, the Takasuka configuration is confirmed to better reproduce deep convective characteristics. Our analysis also identifies several issues that require further refinement of the cloud microphysics scheme, including the representation of weak precipitation and the temperature dependence of snowfall terminal velocity. These results highlight an added value of unprecedented measurement information from EarthCARE Doppler capability that points to a possible area of further improvement of model microphysics in GSRMs at a process level.

 

How to cite: Matsugishi, S., Nakamura, Y., Seiki, T., Roh, W., Suzuki, K., and Satoh, M.: Evaluation of Doppler Velocity in a GSRM Using the EarthCARE Satellite with Implications for Improving Model Cloud Microphysics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16100, https://doi.org/10.5194/egusphere-egu26-16100, 2026.

EGU26-16130 | Posters on site | AS3.11

A new OT detection approach over East Asia and its validation using EarthCARE data 

Jinyeong Kim, Myoung-Hwan Ahn, and Myoung-Seok Suh

Overshooting tops (OTs) are key indicators of severe weather events associated with deep convection, and geostationary satellite observations play a critical role in monitoring OTs with high spatiotemporal resolution. The infrared window texture (IRW-texture) algorithm (Bedka et al., 2010) identifies OTs as localized cold spots relative to the surrounding anvil. This approach overcomes the limitations of traditional brightness temperature difference methods, which tend to overestimate anvil regions as OTs. However, the IRW-texture algorithm involves uncertainties due to its reliance on model-based tropopause information and fixed detection thresholds. To address these limitations, this study proposes a regionally adapted OT detection algorithm for East Asia by incorporating satellite-derived tropopause information from the GK-2A/AMI atmospheric profile product and optimizing key detection thresholds for the target region. The improved algorithm was validated using the Cloud Profiling Radar (CPR) onboard the EarthCARE satellite. The CPR provides enhanced sensitivity and Doppler velocity measurements compared to previous spaceborne radars, enabling precise characterization of the vertical structure of overshooting convection. Taking advantage of these capabilities, we conducted a detailed physical validation of the detected OTs. The results show that the OTs detected by the algorithm align closely with the vertical updrafts captured by the CPR, validating its reliability in identifying active overshooting convection. Although constrained by a limited number of cases, this pioneering validation using EarthCARE observations demonstrates the importance of physically consistent, region-specific adaptations. These results suggest a promising pathway for enhancing next-generation global convection monitoring capabilities.

How to cite: Kim, J., Ahn, M.-H., and Suh, M.-S.: A new OT detection approach over East Asia and its validation using EarthCARE data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16130, https://doi.org/10.5194/egusphere-egu26-16130, 2026.

EGU26-16799 | ECS | Posters on site | AS3.11

Quantifying three-dimensional radiative transfer effects of clouds using EarthCARE observations and collocated airborne data 

Dimitra Kouklaki, Alexandra Tsekeri, Anna Gialitaki, Bernhard Mayer, Silke Groß, Martin Wirth, Claudia Emde, Eleni Marinou, Stelios Kazadzis, and Vassilis Amiridis

The effect of clouds on radiation remains a critical source of uncertainty in climate and weather prediction models. Moreover, the 3D structure of the clouds, including horizontal heterogeneity along with cloud vertical placement, further affects the radiation fields. Herein we utilize the 3D cloud scenes provided by EarthCARE to quantify the effect of the cloud 3D structure on radiation. Monte Carlo radiative transfer (RT) simulations from the MYSTIC/libRadtran model are employed to calculate the 1D vs 3D radiation fields. Airborne observations are also utilized, acquired during the ORCESTRA/PERCUSION EarthCARE Cal/Val campaign in the tropical Atlantic.

Simulated top-of-atmosphere 1D and 3D radiances and irradiances are compared with EarthCARE Broadband Radiometer (BBR) observations, along with collocated radiation observations from the Munich Aerosol Cloud Scanner (specMACS) onboard the HALO aircraft during the ORCESTRA/PERCUSION campaign. The 1D vs 3D RT simulations are performed to investigate the importance of the 3D cloud structure on the cloud radiation fields, for different types of clouds.

This analysis is part of the Obs3RvE EarthCARE+ project, which aims to develop new realistic 3D cloud scenes, combining EarthCARE and Meteosat Third Generation (MTG) observations, employing machine learning tools. These new 3D cloud scenes are expected to improve estimates of the cloud radiative effect from EarthCARE, as well as extend its suite of products to solar energy applications.

 

Acknowledgements:

This work has been financially supported by the Obs3RvE (Optimising 3D RT Earthcare product using geostationary observations and AI) project, funded from the European Space Agency under Contract No. 4000147848/25/I/AG, the PANGEA4CalVal project (Grant Agreement 101079201) funded by the European Union , the CERTAINTY project (Grant Agreement 101137680) funded by Horizon Europe program, the EarthCARE DISC project, funded by the European Space Agency under Contract No. 4000144997/24/I-NS and the AIRSENSE (Aerosol and aerosol cloud Interaction from Remote SENSing Enhancement) project, funded from the European Space Agency under Contract No. 4000142902/23/I-NS. It is also based upon work from COST Action EARLICOST, CA24135, supported by COST (European Cooperation in Science and Technology). DK, ΑΤ and SK would like to acknowledge COST Action HARMONIA (International network for harmonization of atmospheric aerosol retrievals from ground-based photometers), CA21119, supported by COST (European Cooperation in Science and Technology). 

How to cite: Kouklaki, D., Tsekeri, A., Gialitaki, A., Mayer, B., Groß, S., Wirth, M., Emde, C., Marinou, E., Kazadzis, S., and Amiridis, V.: Quantifying three-dimensional radiative transfer effects of clouds using EarthCARE observations and collocated airborne data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16799, https://doi.org/10.5194/egusphere-egu26-16799, 2026.

EGU26-17090 | ECS | Posters on site | AS3.11

EarthCARE Stratospheric Aerosol Optical Depth and Its Impact on ICON Forecast  

Andreas Karipis, Anna Gialitaki, Hao Luo, Johannes Quass, Dimitra Karkani, Alexandra Tsekeri, Athina Argyrouli, Pascal Hedelt, and Vassilis Amiridis

Stratospheric aerosols play a significant role in the Earth’s radiative balance, atmospheric chemistry and large-scale circulation. Despite their importance, vertically constrained stratospheric aerosol optical depth (AOD) fields are not routinely available for use in global climate modelling systems, which therefore continue to rely on climatological background values or total-column AOD information derived from passive remote sensing sensors. To address this limitation, we exploit observations from the EarthCARE mission to derive stratospheric AOD on a global scale following a moderate volcanic eruption and investigate the impact of the eruption induced AOD perturbation through model assimilation.

To this end, we derive the stratospheric AOD at 355 nm from measurements of the EarthCARE/ATLID high-spectral-resolution lidar (HSRL). Stratospheric aerosol layers are identified and constrained utilizing ATLID target classification products. The stratospheric AOD is calculated by vertical integration of the ATLID L2 aerosol extinction profiles and subsequently regridded to the native ICON model grid, producing monthly global fields of stratospheric AOD.

The April 2024 Ruang volcanic eruption is used as the case study to examine the temporal evolution of stratospheric aerosol loading over approximately one year. As EarthCARE was launched two months after the eruption, the early ATLID observations already capture an enhanced stratospheric aerosol load due to the presence of volcanic particles.

Independent HSRL observations at 532 nm from the DQ-1 mission launched in April 2022, are further explored as a complementary data source to bridge multi-spectral, complementary information between the two missions, and support the development of a long-term stratospheric aerosol climatology.

Finally, the impact of assimilating the EarthCARE-derived stratospheric AOD fields into the ICON forecasting system is evaluated. The experiments reveal systematic changes in radiative fluxes and coherent responses in key atmospheric variables, indicating the potential of vertically constrained stratospheric AOD observations assimilation to improve numerical model simulations.

Acknowledgements:

This work has been financially supported by the ACtIon4Cooling (Aerosol Cloud Interactions for Cooling) project, funded from the European Space Agency under Contract No. 4000147715/25/I-LR, the CERTAINTY project (Grant Agreement 101137680) funded by Horizon Europe program, the EarthCARE DISC project, funded by the European Space Agency under Contract No. 4000144997/24/I-NS and the AIRSENSE (Aerosol and aerosol cloud Interaction from Remote SENSing Enhancement) project, funded from the European Space Agency under Contract No. 4000142902/23/I-NS.

How to cite: Karipis, A., Gialitaki, A., Luo, H., Quass, J., Karkani, D., Tsekeri, A., Argyrouli, A., Hedelt, P., and Amiridis, V.: EarthCARE Stratospheric Aerosol Optical Depth and Its Impact on ICON Forecast , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17090, https://doi.org/10.5194/egusphere-egu26-17090, 2026.

EGU26-18995 | Orals | AS3.11

EarthCARE Campaigns Status 

Jonas von Bismarck, Robert Koopman, Alex Hoffmann, Stephanie Rusli, Montserrat Pinol Sole, Malcolm Davidson, Vasileios Tzallas, Bjoern Frommknecht, and Timon Hummel

Assuring the data quality of the ESA’s EarthCARE science products is a comprehensive collaborative effort. It is being realised by contributions from the independent EarthCARE validation team (ECVT) as well as monitoring-, calibration- and airborne campaign activities performed under ESA (co-)management or coordinated with ESA.

Airborne and other field campaigns with EarthCARE-like as well complementary in-situ have payloads have played and continue to play an essential role in stabilizing and improving the quality of the of the EarthCARE’s user products.

EarthCARE is ESA’s most complex Earth Explorer mission to date, in collaboration with JAXA. For the sake of validating the various single and multi-sensor products from the lidar, radar, imager and radiometer,  the number of airborne underflights achieved during EarthCARE’s first 2 years in orbit significantly exceeds those typical for EO missions and is complemented by comparisons with a multitude of ground-based and shipborne instruments worldwide, intercomparisons with other satellites, and analysis involving numerical weather and air quality models. The success of these activities enabled the swift improvement and public release of all scientific EarthCARE products within a year after commissioning.

The presentation will provide the status of EarthCARE campaigns by giving an overview of the activities and selected key findings during its first 2 years in orbit as well as an outlook of what is planned.

How to cite: von Bismarck, J., Koopman, R., Hoffmann, A., Rusli, S., Pinol Sole, M., Davidson, M., Tzallas, V., Frommknecht, B., and Hummel, T.: EarthCARE Campaigns Status, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18995, https://doi.org/10.5194/egusphere-egu26-18995, 2026.

EGU26-20361 | Posters on site | AS3.11

Building a long-term cloud record from spaceborne lidars: merging CALIOP with ATLID 

Artem Feofilov, Karim Slimani, Hélène Chepfer, and Vincent Noël
Clouds exert multifaceted radiative effects on Earth's energy budget, acting as both insulators and reflectors that profoundly influence regional and global climate dynamics. Since 2006, spaceborne active sounders have monitored clouds with unprecedented vertical and horizontal resolution. Yet comparing cloud data from different lidars remains problematic - variations in wavelength, pulse energy, detector type, and observation times create discontinuities that complicate our understanding of long-term cloud behavior.
This study presents a methodology to reconcile cloud observations from multiple spaceborne lidar platforms: CALIPSO (2006–2023), ALADIN/Aeolus (2018–2023), IceSat-2 (2018–present), ACDL/Daqi-1 (2022–present), and ATLID/EarthCARE (2024–present). We have already demonstrated this approach works for CALIOP and ALADIN (Feofilov et al., 2024); here we apply it to bridge CALIOP and ATLID.
 
The approach
We use the Scattering Ratio at 532 nm (SR532) as our common language across all lidars. For measurements at other wavelengths, we convert the retrieved optical properties to SR532 and ATB532 (Attenuated Total Backscatter at 532 nm), enabling direct comparison. Since different signal-to-noise ratios between instruments can affect cloud detection near the detection threshold, we pay close attention to these differences.
When satellites don't share the same viewing times - even with nearly identical equator crossings - we apply a diurnal cycle correction using climatology derived from CATS measurements as in (Feofilov and Stubenrauch, 2019; Feofilov et al., 2014). Since the satellites fly in opposite directions, they observe extratropical zones at different local times, and we must account for this.
For missions that overlap in time, we fine-tune our cloud detection parameters until the datasets transition seamlessly. We then scrutinize collocated data across latitudes, altitudes, and seasons, hunting for differences and correcting for them where we find instrument sensitivity or noise effects.
When instruments don't overlap that is the case for CALIOP and ATLID, we use a different strategy: we identify geographical zones characterized by minimal interannual variability and trends. These "stable" zones become our reference for intercalibration, allowing us to anchor ATLID to CALIOP without a shared observational period.
What we get
We take ATLID's complete baseline, apply the wavelength conversion, perform diurnal cycle corrections, run our detection algorithm with the thresholds we've defined, generate global cloud distributions for the entire mission, and discuss its key properties with respect to CALIOP. 
 
References:
Feofilov, A. G. and Stubenrauch, C. J.: Diurnal variation of high-level clouds from the synergy of AIRS and IASI space-borne infrared sounders, Atmos. Chem. Phys., 19, 13957–13972, https://doi.org/10.5194/acp-19-13957-2019, 2019.
Feofilov, A., Chepfer, H., Noël, V., and Hajiaghazadeh-Roodsari, M.: Towards Establishing a Long-Term Cloud Record from Space-Borne Lidar Observations, Springer aerospace technology, 57–72, https://doi.org/10.1007/978-3-031-53618-2_6, 2024.

How to cite: Feofilov, A., Slimani, K., Chepfer, H., and Noël, V.: Building a long-term cloud record from spaceborne lidars: merging CALIOP with ATLID, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20361, https://doi.org/10.5194/egusphere-egu26-20361, 2026.

EGU26-20488 | ECS | Orals | AS3.11

Cloud characteristics and 3D radiative effects in EarthCARE MSI and synergy retrievals 

Gregor Walter, Anja Hünerbein, Sebastian Bley, and Nils Madenach

Imaging spectrometers, such as the multispectral imager (MSI) onboard EarthCARE, are used to derive cloud properties from backscattered solar radiation. The retrievals rely on the independent column approximation and the assumption of vertically and horizontally homogeneous clouds. These 1D simplificatopns neglect the impact of cloud structure on 3D radiative transfer, leading to biases, e.g., in the derived effective radius or cloud water path of the MSI cloud produt (M-COP).

While MSI provides information on the horizontal cloud field and cloud-top structure from brightness temperatures (BTs), the active instruments of EarthCARE, the cloud profiling radar (CPR) and the atmospheric lidar (ATLID), provide vertical cloud profiles along the satellite track. In the synergy product (ACM-CAP), CPR and ATLID are combined with nadir pixels of MSI to derive best estimates of vertical atmospheric profiles, which serve as a basis for radiative transfer simulations for closure studies in the ESA EarthCARE retrieval chain. As in the single-instrument retrieval, MSI contributes to ACM-CAP under the assumption of independent columns.

In this study, cloud properties from M-COP and ACM-CAP are analyzed while accounting for cloud structure information, including cloud fraction, standard deviations, and BT gradients, which are used to identify whether a pixel is located on the sunlit or shadowy side of a cloud. By comparing sunlit and shadowy pixels, we show that 3D radiative effects introduce systematic biases in both products, with e.g., cloud water path values being higher on the sunlit side. In ACM-CAP, the magnitude of these biases depends on the relative contribution of MSI radiances to each atmospheric column and varies with cloud type and surface conditions.

Cloud properties from M-COP are compared to ACM-CAP to identify patterns of agreement and deviation, with focus on pixels for which we assume low estimated 3D bias in ACM-CAP. Radiative transfer simulations based on ACM-CAP are performed using the MYSTIC Monte Carlo solver, showing aggreement to the observations and demonstrating that the inclusion of MSI radiances in the synergy product introduces 1D/3D inconsistencies that can affect radiative closure studies.

How to cite: Walter, G., Hünerbein, A., Bley, S., and Madenach, N.: Cloud characteristics and 3D radiative effects in EarthCARE MSI and synergy retrievals, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20488, https://doi.org/10.5194/egusphere-egu26-20488, 2026.

EGU26-21727 | ECS | Orals | AS3.11

Global Riming Signatures from EarthCARE CPR Doppler velocity measurements 

Jiseob Kim, Pavlos Kollias, Bernat Puigdomènech Treserras, and Alessandro Battaglia

Riming, the growth of ice particles by accretion of supercooled liquid droplets, is a key microphysical pathway in mixed-phase clouds, strongly influencing precipitation formation and cloud radiative effects. However, its global occurrence and variability have remained poorly constrained by observations, as riming is typically inferred indirectly at the global scale, while more direct evidence has been obtained primarily from limited regions or specific field campaigns. The Earth Cloud, Aerosol and Radiation Explorer (EarthCARE), launched in May 2024, carries the first spaceborne Doppler Cloud Profiling Radar (CPR), enabling near-global measurements of vertical motions within clouds. In this study, we exploit EarthCARE CPR Doppler observations to investigate microphysical signatures embedded in retrieved ice sedimentation velocity, with a particular focus on vertical gradients as an indicator of riming. The physical basis is that rimed ice particles often undergo rapid mass growth over short vertical distances, leading to corresponding changes in fall speed and producing localized acceleration patterns in sedimentation velocity profiles. We develop a gradient-based riming detection algorithm to derive riming probability at near-global scale and present the first maps of its spatial distribution and seasonal variability. The resulting climatology reveals where riming is most prevalent and how its occurrence shifts with season, providing observational constraints that were previously inaccessible from space. Because riming remains a major source of uncertainty in weather and climate model microphysics, these global statistics offer a new benchmark for evaluating and improving riming parameterizations in numerical models, including emerging km-scale modeling efforts.

How to cite: Kim, J., Kollias, P., Puigdomènech Treserras, B., and Battaglia, A.: Global Riming Signatures from EarthCARE CPR Doppler velocity measurements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21727, https://doi.org/10.5194/egusphere-egu26-21727, 2026.

EGU26-22091 * | Orals | AS3.11 | Highlight

EarthCARE Mission Status 

Bjoern Frommknecht and the EarthCARE Mission Team

The Earth Cloud Aerosol and Radiation Explorer (EarthCARE) mission, a collaborative effort between the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA), aims to address critical uncertainties in climate predictions related to cloud-aerosol interactions and their effects on solar and thermal radiation.

Launched in May 2024, EarthCARE has been in orbit for almost two years, providing invaluable data to the scientific community. EarthCARE's payload includes two active instruments, the cloud-aerosol lidar (ATLID) and the cloud Doppler radar (CPR), along with the passive multispectral imager (MSI) and broad-band radiometer (BBR). These instruments work synergistically to deliver vertical profiles of cloud ice and liquid water, aerosol types, precipitation, and heating rates. Additionally, they measure solar and thermal top-of-atmosphere radiances, aiming to reconstruct top-of-the-atmosphere short- and longwave fluxes with an accuracy of 10 Wm-2 on a 10 km x 10 km scene. The mission has successfully developed and disseminated data products through a coordinated approach between ESA and JAXA, ensuring continuous information exchange between European and Japanese algorithm and science teams. EarthCARE data is freely available to the scientific community, with all products available to the public, including three- and four-sensor Level-2b synergistic data.

This presentation gives the EarthCARE mission status after almost 2 years in orbit. It will cover the status of all mission elements, including instruments, platform and ground segments. In addition highlight results from the mission will be shown, together with an outlook on future activities.

How to cite: Frommknecht, B. and the EarthCARE Mission Team: EarthCARE Mission Status, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22091, https://doi.org/10.5194/egusphere-egu26-22091, 2026.

Irrigation water management is a critical factor that influences crop biomass, yield, and water usage, since irrigation makes the crop development independent of rainfall. Poor irrigation management can result in many problems on the farm and off the farm, such as waterlogging, erosion, and non-point source pollution. Therefore, improving irrigation water-use-efficiency is essential to reduce the amount of water needed without penalizing the yields. Considering the growing competition for water resources, there is a need to explore novel methods for quantifying and enhancing water use efficiency in irrigated fields, such as Unmanned Aerial Vehicle (UAV)-based remote sensing. This study integrates UAV-derived vegetation indices with machine-learning (ML) algorithms to quantify biomass and yield response of rice under alternate wetting and drying (AWD) and wheat under different irrigation methods (drip, sprinkler, and flood) with variable rates of crop evapotranspiration (100%, 75%, 50% and 0% rainfed treatment) across two seasons of the rice-wheat cropping system in Roorkee, India. The biomass and yield results obtained from the different ML algorithms were compared. During the training process of the ensemble random forest model, it performed better with a higher KGE (0.91) and a lower value of NRMSE (0.033), and a minimal PBIAS of 0.13%. The ensemble random forest model performed better during the testing process of the rice yield estimation (R2 = 0.60, KGE = 0.71, PBIAS = −2.26%, NRMSE = 0.136). For wheat yield estimation, training results were similar with strong model performance (R2 = 0.8137, KGE = 0.83, PBIAS = 1.36%, NRMSE = 0.470). The UAV-ML workflow captured both the fine-scale spatial variability needed for site-specific field decisions and the process understanding needed for generalization across the seasons. This integrated workflow supports the UN Sustainable Development Goals (SDGs), specifically SDG 2 (Zero Hunger) and SDG 6 (Clean Water and Sanitation).

How to cite: Kumar Vishwakarma, S., Kothari, K., and Pandey, A.: Spatial Mapping of Biomass and Yield of Rice-Wheat Cropping Systems across Different Irrigation Methods Using UAV Images and Machine Learning Algorithms , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-452, https://doi.org/10.5194/egusphere-egu26-452, 2026.

EGU26-1139 | PICO | HS6.7

Floodalyzer: A QGIS Plugin for Accessible and Rapid Flood Event Assessment 

Luisa Fuest and Antara Dasgupta

Floods are among the most devastating natural disasters, causing significant loss of life and economic damage. As extreme flood events become more frequent, rapid and accessible flood analysis tools are crucial in guiding early recovery efforts. This study presents the QGIS plugin ‘Floodalyzer’ developed to provide a quick and easy workflow for flood event analysis. By automating the processing and visualization of flood extent data from the Global Flood Monitoring System (GFM), derived from remote sensing, in combination with building footprints from various data sources, the plugin enables users to analyze past flood events without requiring expert knowledge or expensive proprietary software.

Floodalyzer operates within the widely used open-source GIS platform QGIS, making it highly accessible. Users manually download raster data and shapefiles from the web, which serve as inputs for automated analysis. The plugin then processes the data and generates output files, including a shapefile showing which buildings were flooded and for how long. Additionally, it compiles a HTML report including graphs that further describe the area of interest and summarize the plugin’s results (e.g. Building Footprint Heatmap, Observed Flood Extent Raster Calendar Display, Flooded Area Duration Bar Chart). The effectiveness of the tool was evaluated using case studies in Pakistan and Germany, where results were compared against CEMS’s Rapid Mapping Product. The CEMS product was not captured at the time of maximum flooding and therefore shows smaller inundated areas in many places compared to the plugin’s results. However, the locations and overall shapes of the flooded areas are generally consistent.

The case studies highlight the unique selling point of Floodalyzer – it’s ability to process flood extent data over extended time periods to analyze flood duration and damage, which enables a more comprehensive analysis of the available data. At the same time the results highlight uncertainties in flood extent, primarily originating from the GFM input data. Large exclusion mask areas indicate zones of high uncertainty, especially in urban environments where flood detection is more challenging. Temporal uncertainties also arise from gaps in satellite coverage, limiting data availability, especially in regions between the tropics.

Future improvements will focus on reducing runtime, and integrating statistical uncertainty assessments in the plugin’s output with human-readable explanations. Further, automated GFM data retrieval from the Global Flood Awareness System automating the download of the flood masks given an input AOI, would eliminate the need for manual downloads and thereby streamline the analysis process. By bridging the gap between high, complex data amounts and the need for a rapid response to flooding events, this tool provides decision-makers with a sound basis for dealing with the impacts of flooding in the response and recovery phase. Floodalyzer thus supports improved flood management through broader uptake of remotely sensed flood information, by lowering barriers to accessibility for flood extent data.

How to cite: Fuest, L. and Dasgupta, A.: Floodalyzer: A QGIS Plugin for Accessible and Rapid Flood Event Assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1139, https://doi.org/10.5194/egusphere-egu26-1139, 2026.

Extreme rainfall events have become more frequent and intense under climate change, presenting increasing challenges for hydrological monitoring and flood risk management. High-resolution rainfall observations are essential for capturing the spatial and temporal variability of storm events, yet conventional rain-gauge networks suffer from limited spatial coverage and cannot resolve rapidly evolving convective structures. Moreover, high-intensity rainfall events are inherently rare in natural settings, resulting in data gaps in upper rainfall categories. To address this limitation, we integrate natural rainfall observations with controlled artificial rainfall experiments to construct a comprehensive and balanced multi-class dataset covering 0–70 mm/hr at 5 mm/hr intervals. We develop a multimodal deep learning framework that jointly leverages rainfall imagery and acoustic measurements for rainfall-intensity estimation. The two sensing modalities provide complementary physical information: imagery captures streak morphology, drop density, and spatial distribution patterns, while acoustics encode drop momentum, kinetic energy, and impact signatures. Neither modality alone fully characterizes rainfall processes across all intensity ranges; by combining them, the model benefits from richer and more discriminative features. Two-second audio segments are converted into log-mel spectrograms, and a Cross-Attention fusion mechanism enables the network to selectively emphasize the most informative cues from each modality for different rainfall categories. Image-based data augmentation such as horizontal flipping further expands the training space and improves model generalization.

Compared with previous studies that relied on single-modality inputs or coarse categorical schemes, our framework achieves a substantially finer classification resolution (0–70 mm/hr in 5-mm/hr bins) and exhibits improved discrimination between adjacent intensity levels. The multimodal architecture consistently outperforms single-modality baselines, with the performance gains being particularly notable in the moderate-to-heavy rainfall range, where the model achieves higher classification accuracy, highlighting the benefits of true cross-modal complementarity. The integration of artificial and natural rainfall further produces a balanced and physically representative dataset that captures both controlled high-intensity scenarios and real-world variability.Overall, this study demonstrates the potential of multimodal sensing and deep learning to advance rainfall monitoring capabilities. The proposed non-contact, low-cost, and high-resolution approach offers a promising pathway for enhancing rainfall observation in regions with sparse gauge coverage, strengthening flood early warning systems, and supporting real-time hydrological applications under a changing climate.

How to cite: Lin, C.-C. and Ho, H.-C.: Cross-Attention Multimodal Learning Using Image and Audio for Rainfall Intensity Estimation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2660, https://doi.org/10.5194/egusphere-egu26-2660, 2026.

EGU26-10725 | ECS | PICO | HS6.7

On the optimisation of numerical weather prediction model configuration for improved flood forecasting 

Elena Leonarduzzi, Katrin Ehlert, David Leutwyler, and Massimiliano Zappa

Hydrological forecasts are essential for the timely and accurate prediction of flooding events, which are among the most impactful natural hazards for both infrastructure and human life in Europe and many other regions worldwide. Most existing flood warning systems are supported by hydrological models. Their accuracy depends not only on the representativeness and proper calibration (when required) of the model itself, but also on the quality of its inputs. While static inputs, particularly soil parameters, are highly uncertain, weather forecasts are arguably the most influential drivers.

In this study, we recreate the entire operational modelling framework used in Switzerland. Weather forecasts are provided by ICON (MeteoSwiss) and are used as input for WaSiM (FOEN), which produces streamflow predictions and issues warnings when necessary. We focus on several case studies, including selected catchments (e.g., Thur) and historical events that exceeded national flood warning levels (e.g., 30 May–2 June 2024).

This setup allows us to experiment with different configurations of the numerical weather prediction (NWP) model and to assess their downstream impacts on hydrological forecasts. We test different lead times to evaluate how early flood peaks can be detected, varying ensemble sizes to determine how many members are required to capture “extreme” flooding scenarios, and different spatial resolutions (500m – 2km) to assess the impact of resolving small-scale processes (e.g., convection).

Model performance is evaluated using classical hydrological metrics (NSE, KGE, RMSE, etc.), as well as more operationally relevant metrics for warning systems, such as whether thresholds are exceeded, how early exceedances occur, and their duration. Finally, we test different products for initializing model runs, either interpolated station-based products or NWP analysis products and assess the influence of the hydrological model itself through a sensitivity analysis of its parameters.

The results of this study will shed light on how NWP model configurations affect flood forecasting and, in turn, improve flood early warning design and decision-making.

How to cite: Leonarduzzi, E., Ehlert, K., Leutwyler, D., and Zappa, M.: On the optimisation of numerical weather prediction model configuration for improved flood forecasting, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10725, https://doi.org/10.5194/egusphere-egu26-10725, 2026.

EGU26-15447 | ECS | PICO | HS6.7

Remote sensing–based urban floodplain mapping: the added value of UAV-LiDAR compared to global and GNSS-derived DEMs 

Eduardo Luceiro Santana, Laura Martins Bueno, Gabriel Souza da Paz, Rafael De Oliveira Alves, Tamara Leitzke Caldeira, Samuel Beskow, Aryane Araujo Rodrigues, Julio Cesar Angelo Borges, Denis Leal Teixeira, Gustavo Adolfo Karow Weber, and Diuliana Leandro

Flood risk management in urban floodplains strongly depends on the spatial resolution of digital elevation models (DEMs), which control floodplain connectivity, flow pathways, and surface storage. In many developing countries, flood-related studies rely predominantly on publicly available global DEM products, whose spatial resolution and vertical accuracy are often insufficient to represent subtle topographic gradients, densely vegetated floodplains, and complex urban microtopography. These limitations are particularly critical in low-relief environments, where small elevation differences exert a disproportionate control on inundation extent and flood dynamics. This issue has become increasingly evident in subtropical lowland regions of southern Brazil, where extreme flood events in 2023–2024 exposed shortcomings of commonly used global DEMs for urban floodplain applications. Therefore, the Piratini River watershed has been the focus of ongoing efforts to develop a real-time hydrological forecasting system to support decision-making during flood emergencies under data-scarce conditions. The urban areas of Pedro Osório and Cerrito along the main floodplain of the Piratini River constitute the core operational domain of this system and are recurrently affected by flooding. The watershed drains approximately 4,700 km² upstream of the municipalities and is characterized by low relief and wide floodplains. This study investigates the applicability of publicly available global DEMs and locally derived high-resolution elevation datasets for floodplain mapping and hydrological–hydrodynamic applications in these urban areas. A comparative assessment was conducted using two global DEM products - ALOS PALSAR (12.5 m) and ANADEM (30 m) - and three locally derived DEMs generated from high-resolution surveys. Local datasets include two Global Navigation Satellite System (GNSS) Real-Time Kinematic (RTK)–based surveys (static and kinematic) acquired with an Emlid Reach RS2+ receiver using real-time corrections via NTRIP (Networked Transport of RTCM via Internet Protocol), and an unmanned aerial vehicle (UAV)–based Light Detection and Ranging (LiDAR) survey acquired with a DJI Matrice 350 RTK platform equipped with a Zenmuse L2 sensor. The static GNSS survey comprised 2,921 points, while the kinematic survey yielded approximately 34,000 at a 1-s sampling interval. The UAV–LiDAR survey covered 21.5 km² of the urban floodplain. Raw elevation data from local surveys were converted from ellipsoidal to orthometric altitude using the hgeoHNOR2020 geoid model. GNSS-derived altitudes were interpolated using ordinary kriging in ArcGIS Pro. LiDAR data were processed in DJI Terra, resulting in a high-density point cloud (> 98 points m⁻²) and a terrain model with decimetric spatial resolution. Results reveal clear differences among datasets. Global DEMs show limited capability to represent floodplain connectivity and microtopography, particularly in vegetated areas. GNSS RTK–based DEMs provide intermediate performance but are constrained by survey logistics and GNSS signal degradation. In contrast, the UAV-based LiDAR DEM provides the most detailed and hydrologically meaningful representation of floodplain morphology, including vegetated and off-street areas, enabling improved delineation of flow paths and floodplain storage. These findings highlight the critical role of high-resolution elevation data for floodplain mapping and hydrological–hydrodynamic analyses in low-relief urban environments, reinforcing UAV-based LiDAR as a key remote sensing tool for risk assessment and climate adaptation in data-scarce regions.

How to cite: Luceiro Santana, E., Martins Bueno, L., Souza da Paz, G., De Oliveira Alves, R., Leitzke Caldeira, T., Beskow, S., Araujo Rodrigues, A., Angelo Borges, J. C., Leal Teixeira, D., Adolfo Karow Weber, G., and Leandro, D.: Remote sensing–based urban floodplain mapping: the added value of UAV-LiDAR compared to global and GNSS-derived DEMs, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15447, https://doi.org/10.5194/egusphere-egu26-15447, 2026.

Flood risk assessment and capturing complex inundation dynamics increasingly relies on high-resolution Earth observation data and artificial intelligence (AI). This study presents a AI-driven geospatial framework for integrated flood susceptibility mapping and wet-season surface water persistence analysis. Flood susceptibility is quantified using machine-learning and deep-learning models trained on multi-source environmental predictors.  A long-term satellite time series are analyzed to derive spatial metrics of surface water frequency and persistence.

Results demonstrate that integrating surface water persistence substantially enhances the interpretation of AI-based flood susceptibility maps. It provides added value for flood risk assessment and management compared to event-based mapping alone. The proposed framework contributes to next-generation flood risk monitoring by coupling remote sensing, AI, and temporal hydrologic information, and offers a transferable foundation for data-driven flood management and decision support under increasing climate variability.

 

 

How to cite: Golmohammadi, G. and Tziolas, N.: Integrating Flood Susceptibility and Surface Water Persistence Using Geospatial AI for Flood Risk Monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15771, https://doi.org/10.5194/egusphere-egu26-15771, 2026.

Earthquakes can cause rapid changes in elevation and topographic relief, which, in turn, affect hydrologic regimes and modify flood risk in affected regions. The regulatory floodplain, an area of elevated flood hazard adjacent to water bodies, is critical for managing exposure and mitigating flood risk in nations. Shifts in the distribution of flood risk in regions impacted by seismic activity constitute a compound hazard. Tools are needed to enable reevaluation of regulatory flood maps after seismic events, minimizing exposure of affected populations to additional flood risk. In the United States, floodplain mapping is primarily implemented by the Federal Emergency Management Agency (FEMA), known as regulatory flood mapping. They are based on Hydraulic modeling and delineate the floodplain for areas representing a 1% annual chance of flooding. The floodplain map is not updated regularly by FEMA; it relies on manual, costly revision processes and does not consistently use current, high-resolution, and up-to-date elevation data. Therefore, these maps will struggle to detect recent flood behavior, thereby increasing flood risks and limiting the effectiveness of regulatory flood mapping management. This study presents a rapid, satelliteintegrated framework for updating regulatory flood maps in regions exposed to topographic shifts from earthquakes. Using the 2019 Ridgecrest earthquake sequence as a case study in the North and South Fork Kern River basin, California. Specifically, we used the U.S Geological Survey 3DEP/NED with 10-m resolution DEM, which represented the pre-earthquake topography, integrated with a vertical displacement data derived from InSAR time series analysis to generate a corrected post-earthquake DEM. Both DEMs were then used in the HEC-RAS model to quantify changes in floodplain extent and inundation patterns under multiple return-period scenarios. To assess model performance and quantify the accuracy improvements in regulatory flood mapping, observed flood inundation maps derived from high-resolution PlanetScope satellite imagery were used in the validation. Our integrated approach demonstrates how InSAR-updated topography improves floodplain mapping accuracy and enables rapid updates to regulatory flood maps. HEC-RAS modeling results across three reaches along the North and South Fork Kern River consistently showed larger flood extents in post-earthquake simulations relative to pre-earthquake conditions. Validation using PlanetScope-derived flood inundation maps demonstrates improved model performance for the post-earthquake DEM, with an F-score 84.52% compared to pre-earthquake simulations, using an optimal NDWI threshold of 0.35.

How to cite: Al-Amry, N. and Carter, E.: Assessing Fluvial Flood Risk Changes Using an Updated Digital Elevation Model Post-Earthquake: A Case Study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15883, https://doi.org/10.5194/egusphere-egu26-15883, 2026.

EGU26-16153 | ECS | PICO | HS6.7

Virtual Reality–Based Visualization of Urban Flood Dynamics Using SWMM 

Jiye Park, Minjeong Cho, Gihun Bang, Minhyuk Jeung, Daeun Yun, and Sang-Soo Baek

Urban flooding and water pollution have become increasingly severe challenges worldwide as a result of climate change and rapid urbanization, posing substantial risks to public safety, urban infrastructure, and environmental quality (Mark et al., 2004; Andrade et al., 2018). Intense rainfall events frequently exceed the capacity of urban drainage systems, leading to surface inundation and the transport of pollutants into receiving water bodies. To address these issues, numerical hydrological and hydraulic models have been widely applied to simulate urban runoff processes, sewer network performance, and water quality dynamics. Among these models, the Storm Water Management Model (SWMM) is one of the most commonly used tools for analyzing urban drainage systems and pollutant transport under various rainfall scenarios (Gironás et al., 2010). Despite its widespread adoption and robust modeling capabilities, SWMM primarily presents simulation outputs in the form of numerical tables and two-dimensional graphs. This conventional output format limits intuitive interpretation and restricts the ability to analyze spatial and temporal flood dynamics within complex urban environments (Zhang et al., 2016). This study proposes a virtual reality (VR)–based visualization framework that integrates SWMM simulation results with the Unity game engine to enhance the interpretability of urban flooding and water quality simulations. In the proposed framework, rainfall–runoff processes, inundation depth, and pollutant diffusion are first simulated using SWMM for a selected urban catchment. The resulting hydrological and hydraulic outputs are then converted into data formats compatible with the Unity environment. A three-dimensional urban model is constructed to represent surface topography and drainage infrastructure, enabling the visualization of flooding processes in a spatially explicit manner. Flood extent and water depth are visualized dynamically within the virtual environment, allowing users to observe flood propagation over time. In addition, pollutant transport is represented using color-based visualization techniques, where variations in color indicate changes in pollutant concentration. This approach provides an intuitive representation of water quality degradation during flood events. The VR system supports interactive exploration through the use of head-mounted displays and motion interfaces, enabling users to navigate the virtual urban space and examine flooding and pollution patterns from multiple perspectives. The immersive nature of the VR environment enhances spatial perception and facilitates a more comprehensive understanding of complex flood processes compared to traditional two-dimensional visualization methods. By allowing users to directly experience simulated flood scenarios, the proposed framework supports more effective interpretation of model results and improves communication of flood risk information. The results of this study demonstrate that VR-based visualization has significant potential as a decision-support tool for urban flood risk assessment, emergency response planning, and disaster management training.

How to cite: Park, J., Cho, M., Bang, G., Jeung, M., Yun, D., and Baek, S.-S.: Virtual Reality–Based Visualization of Urban Flood Dynamics Using SWMM, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16153, https://doi.org/10.5194/egusphere-egu26-16153, 2026.

The accelerating impacts of climate change and subsequent impact on urban environments such as flooding risks, extreme heat and heavy rain, necessitate rapid and integrated planning strategies. Urban Digital Twins (UDT) have emerged as valuable tools, offering the ability to dynamically model, simulate, and visualize complex processes to support data-driven decision-making. However, a comprehensive strategy that supports the integration of the multitude of UDTs that is being developed specifically into climate adaptation measures, while ensuring interoperability, digital sovereignty and stakeholder participation, is still lacking.

This contribution introduces the collaborative project LINKUDT (“Coordination and Collaboration Platforms for the Synergetic Conception, Development, Interoperability, and Digital Sovereignty of Urban Digital Twins”). Funded by the German Federal Ministry of Research, Technology and Space for a duration of 48 months, LINKUDT serves as the overarching companion research project for six regional real-world laboratories across Germany. The primary objective of the project is to establish UDTs as central instruments for speeding up urban planning processes to improve climate adaptation and sustainable urban development by identifying synergies and supporting interoperability.

A core challenge addressed by LINKUDT is the creation of interoperable and sustainable data infrastructures. Following the FAIR principles (Findable, Accessible, Interoperable, Reusable), the project aims at advancing standards that allow for the efficient integration of heterogeneous data sources, such as sensor networks and environmental models. To prevent vendor lock-in and ensure long-term data portability, LINKUDT emphasizes digital sovereignty through the use and further development of open-source software modules and standards (e.g., OGC API Processes, SensorThings API, CityGML).

Further key outcomes of LINKUDT include training modules for stakeholders /e.g. public administration, developers), and policy recommendations for the nationwide application of digital twin technologies.

By linking the National Research Data Infrastructure for Earth System Sciences (NFDI4Earth) with administrative data infrastructures (GDI-DE), LINKUDT creates a scalable model for evidence-based urban governance. 

With our contribution we aim to reach out to further digital twin initiatives related to climate change to initiate further exchange on interoperability, digital sovereignty and emerging technologies.

How to cite: Jirka, S., Radtke, J., and Reiß, J.: LINK Urban Digital Twinning (LINKUDT): Advancing Climate Adaptation and Planning Acceleration through Interoperable Digital Twin Ecosystems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17814, https://doi.org/10.5194/egusphere-egu26-17814, 2026.

Non-contact river monitoring is essential for understanding hydraulic phenomena and providing real-time disaster mitigation information during large-scale floods. Our previous research (Yorozuya et al., 2026) developed a method to inversely estimate riverbed elevation by integrating UAV-derived surface velocity (via PIV) and water surface geometry (via LiDAR) into a Physics-Informed Neural Networks (PINNs) framework using automatic differentiation of the governing equations. However, that approach relied on a uniform velocity correction factor across the entire reach, which led to significant underestimations of water depth in complex flow fields, such as those near spur dikes.

In this study, we propose an enhanced estimation algorithm that incorporates secondary flow effects into the momentum equations to improve bathymetric accuracy. Following the methodology of Iwasaki et al. (2013), we identify regions where surface velocity vectors exhibit curvature and account for the resultant increase in flow resistance. This approach aims to correctly identify water depth even in regions where surface velocities are low but hydraulic complexity is high.

Field experiments were conducted in a reach of the Kurobe River (bed slope ≈1/100, 20m wide by 50m long), characterized by a spur dike in the center of the domain. High-resolution water surface geometry and velocity fields were captured using a UAV-mounted LiDAR (DJI Zenmuse L2) and a photogrammetric camera (P1). These data were integrated into the PINNs loss functions, which were defined based on the continuity equation, the shallow water equations, and the conservation of discharge across cross-sections.

The results demonstrated a marked improvement in estimation reliability, particularly in the separation zones downstream of the spur dike. Without secondary flow considerations, the model estimated near-zero water depth in large wake vortices due to the low surface velocities. By incorporating secondary flow effects, the model correctly evaluated the increased apparent roughness due to flow curvature, yielding deeper and more accurate bathymetry consistent with ground-truth data obtained by boat-mounted ADCP. This study highlights the potential of using only UAV-based remote sensing to achieve high-precision bathymetric inversion in morphologically complex river environments.

Iwasaki, T., Shimizu, Y., and Kimura, I. (2013). An influence of modeling of secondary flows to simulation of free bars in rivers. Journal of Japan Society of Civil Engineers, Ser. B1 (Hydraulic Engineering), Vol. 69, No. 3, 147–163.

Yorozuya et al. (2016) Seeing the unseen, RiverFlow2026 (Under review)

How to cite: Yorozuya, A., Inaba, R., and Kudo, S.: Bathymetry Estimation in Complex River Morphology using UAV-based Remote Sensing and Physics-Informed Neural Networks Incorporating Secondary Flow Effects, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17859, https://doi.org/10.5194/egusphere-egu26-17859, 2026.

LiDAR-derived digital elevation models (DEMs) are increasingly adopted in hydrodynamic flood modelling; however, their direct use, particularly in complex urban environments, remains problematic. Although LiDAR provides high-resolution surface information and supports the generation of bare-earth digital terrain models (DTMs), unresolved flow-permeable structures such as bridges, culverts, and elevated transport infrastructure, together with micro-scale urban features including narrow river channels, pathways, kerbs, and missing submerged channel bathymetry, systematically distort flow connectivity and channel conveyance. These deficiencies introduce structural biases into flood simulations, yet existing studies typically address individual features in isolation, limiting transferability and large-scale applicability.

This study reframes LiDAR DEM preprocessing as a process-based investigation into how unresolved terrain features bias flood hydraulics and introduces an automated, physically consistent terrain reconstruction framework that explicitly targets these bias mechanisms. The framework is implemented at the national scale using the 2 m LiDAR-derived DTM for England.

Three dominant sources of hydrodynamic bias are addressed. First, flow-permeable structures, including bridges, culverts, and elevated transport infrastructure, are systematically identified using observed water surface information and river network data, and the terrain beneath these structures is reconstructed using interpolation-based techniques to restore hydraulic connectivity. Second, impermeable urban features, such as buildings and kerbs, are selectively elevated while preserving longitudinal connectivity along roads and pathways, ensuring realistic overland flow routing. Third, submerged river bathymetry is reconstructed using empirical relationships between river width and water depth to recover channel conveyance absent from bare-earth DTMs.

The resulting terrain dataset is directly applicable to hydrodynamic flood modelling without manual intervention. Sensitivity analyses across multiple historical flood events demonstrate that restoring flow connectivity and reconstructing channel bathymetry exert distinct and flow-regime-dependent controls on simulated flood extent, water levels, and discharge. In particular, unresolved flow-permeable structures predominantly govern urban inundation patterns, whereas missing bathymetry represents the primary source of error in channel hydraulics.

By systematically isolating and correcting key terrain-induced bias mechanisms, this study provides generalisable insights into the process sensitivity of catchment and urban flood models to DEM representation and offers a scalable pathway for improving large-scale flood simulations using LiDAR data.

How to cite: Chen, H., Tong, X., and Liang, Q.: Reconstructing Flow Connectivity and Channel Conveyance in LiDAR-Derived Terrain for National-Scale High-Resolution Flood Modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22261, https://doi.org/10.5194/egusphere-egu26-22261, 2026.

GI5 – Investigation Methods for Surface and Subsurface

EGU26-3143 | Posters on site | GI5.1

PAC, a User-Friendly App for Hybrid Active-Passive MASW along Linear Geotechnical Infrastructures: Application to Advanced Seismic Diagnosis of Railway Embankments 

Ludovic Bodet, José Cunha Teixeira, Audrey Burzawa, Marine Dangeard, Amélie Hallier, Joséphine Boisson Gaboriau, and Amine Dhemaied

In a context where low-carbon transport is becoming increasingly essential, the diagnosis and maintenance of railway infrastructure have become critical issues. Current assessment techniques still rely heavily on destructive testing of embankments, sublayers, and underlying soils. These structures are also exposed to more frequent and less predictable extreme weather events, threatening their mechanical integrity and long-term stability. High-density, high-resolution geophysical methods therefore offer a compelling non-destructive alternative, particularly for characterizing and monitoring the mechanical properties of soils. Over the past decade, major advances have been made in seismic acquisition, processing, and interpretation. We present an overview of our recent contributions, mainly based on surface wave-methods, which require low energy sources and are well suited to railway environments (Cunha Teixeira et al., 2025a). We have developed high-efficiency acquisition strategies using landstreamers, combined with conventional active sources (weight drop or hammer) and passive sources (induced by trains or traffic). We present PAC (Cunha Teixeira et al., 2025b), a user-friendly application designed for processing multichannel analysis of surface waves (MASW). It integrates stacking and interferometry-based approaches to extract multimodal dispersion images, enabling the detection of lateral variations within embankments or continuous site monitoring. Deep learning supports semi-automatic picking, while Bayesian inversion (Burzawa et al., 2025) facilitates the interpretation of mechanical models and aids reliable decision-making in railway infrastructure management.

References:

Burzawa, A., Bodet, L., Dangeard, M., Barrett, B., Byrne, D., Whitehead, R., Chaptal, C., Cunha Teixeira, J., Cárdenas, J., Sanchez Gonzalez, R., Eriksen, A., Dhemaied, A. (2025). Efficient mechanical evaluation of railway earthworks using a towed seismic array and Bayesian inference of MASW data. arXiv preprint https://doi.org/10.48550/arXiv.2507.16491

Cunha Teixeira, J., Bodet, L., Rivière, A., Solazzi, S.G., Hallier, A., Gesret, A., El Janyani, S., Dangeard, M., Dhemaied, A., Boisson Gaboriau, J. (2025a). Neural machine translation of seismic ambient noise for soil nature and water saturation characterization. Geophysical Research Letters, 52(13) https://doi.org/10.1029/2025GL114852

Cunha Teixeira, J., Burzawa, A., Bodet, L., Hallier, A., Decker, B., Lin, F., Dangeard, M., Boisson Gaboriau, J., & Dhemaied, A. (2025b). Passive and Active Computation of MASW (PAC). Zenodo. https://doi.org/10.5281/zenodo.17639980

How to cite: Bodet, L., Cunha Teixeira, J., Burzawa, A., Dangeard, M., Hallier, A., Boisson Gaboriau, J., and Dhemaied, A.: PAC, a User-Friendly App for Hybrid Active-Passive MASW along Linear Geotechnical Infrastructures: Application to Advanced Seismic Diagnosis of Railway Embankments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3143, https://doi.org/10.5194/egusphere-egu26-3143, 2026.

EGU26-3235 | Posters on site | GI5.1

Case study: Integrated interpretation of borehole acoustic televiewer (ATV) and radar data for imaging major fracture networks in crystalline rock 

Janghwan Uhm, Yeonguk Jo, Woong Kang, Taejong Lee, and Jung-Wook Park

Characterizing fracture networks in deep (hundreds-of-meters) crystalline rock is a key requirement for assessing the suitability of a high-level radioactive waste repository site. Hydraulically conductive fracture networks may act as preferential groundwater pathways and therefore need to be identified for long-term safety assessment. In line with the geophysical exploration objective to investigate and visualize connected fracture networks in deep rock, this study proposes an integrated interpretation strategy combining borehole-based multi geophysical data systems. This work is part of a basic research project of the Korea Institute of Geoscience and Mineral Resources (KIGAM) entitled “Development of Core Technologies for Characterization and Modeling of Fractured Rock in the Assessment of Site Suitability for High-Level Radioactive Waste Disposal”.

This study aims to identify and quantitatively characterize major fracture-network intervals around the borehole by integrating acoustic televiewer (ATV) borehole imaging logs with borehole radar data. ATV provides high-resolution structural information for fractures penetrating the borehole wall, including dip, dip direction, and aperture (where resolvable). However, because ATV observation is confined to the borehole wall image, it has limited capability to evaluate the continuity and spatial distribution of the fractures around the borehole. In contrast, while quantitative characterization of detailed fracture geometry (e.g., orientation and aperture) from borehole radar data alone is difficult, it can image relatively large and continuous fractures within approximately 10-15 m of the borehole that may be hydraulically conductive. Borehole radar method can also detect fractures that do not directly intersect the borehole. Using these complementary strengths, we propose the joint interpretation strategy to image major fracture-network candidates around borehole and to infer their dip, dip direction, aperture, and relative continuity. In addition, we demonstrate the workflow through a case study with field data.

The case study was conducted using ATV and borehole radar datasets acquired from a KIGAM borehole down to a depth of 100 m. First, based on the ATV log, fracture characteristics (e.g., dip, dip direction, and aperture) were analyzed, and major fracture-network intervals with clustered fractures were identified. Then, near-borehole (early-time) reflection events in the borehole radar data were analyzed to evaluate their relationship with the major fracture-network intervals derived from the ATV log. In particular, distinct reflectors observed at relatively later times (i.e., beyond the near-borehole) in radar data were matched to the major fracture-network intervals derived from ATV to estimate the relative continuity of them around the borehole. The proposed borehole-based integrated ATV and radar interpretation strategy enables characterization of major fracture networks and is expected to provide a practical approach for screening and visualizing deep fracture networks associated with the stability of repository sites.

How to cite: Uhm, J., Jo, Y., Kang, W., Lee, T., and Park, J.-W.: Case study: Integrated interpretation of borehole acoustic televiewer (ATV) and radar data for imaging major fracture networks in crystalline rock, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3235, https://doi.org/10.5194/egusphere-egu26-3235, 2026.

EGU26-4222 | Orals | GI5.1

Soil-structure interaction issues in complex environments: the example of a 250 m high chimney. 

Giorgio Cassiani, Letizia Nardi, Ilaria Barone, Mirko Pavoni, Jacopo Boaga, Antonio Fuggi, Mohamed Elghasti, and Alessandro Brovelli

Soil-structure interactions must be properly accounted for also in the assessment of structure vulnerability to seismic inputs. This is particularly true in the case of very large structures where the vibrational response of the structure itself can propagate to the soil also under standard conditions, when the characterization of the soil response is generally carried out. In this contribution we demonstrate how only an integrated approach making use of all available soil characterization techniques (namely MASW, ReMi and HVSR) allows for a correct analysis of the recorded data, eliminating the effects caused by the vibrations caused by the structure itself, and thus focusing only on the soil response itself. In absence of such data integration, directional noise coming from the structure vibration itself may cause gross misunderstanding of the soil characteristics both in terms of soil Vs and natural frequency.

How to cite: Cassiani, G., Nardi, L., Barone, I., Pavoni, M., Boaga, J., Fuggi, A., Elghasti, M., and Brovelli, A.: Soil-structure interaction issues in complex environments: the example of a 250 m high chimney., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4222, https://doi.org/10.5194/egusphere-egu26-4222, 2026.

EGU26-4950 * | Orals | GI5.1 | Highlight

Deep Electrical Resistivity Tomography (DERT) in the Campi Flegrei area (Naples, Italy) 

Enzo Rizzo, Sabatino Piscitelli, Francesco Stigliano, and Vincenzo Lapenna and the Working group MS-Campi Flegrei project of CNR (IGAG-IMAA)

Within the activities of the Geophysical Prospecting Unit (UR2) of the MS Campi Flegrei project, funded by the Department of Civil Protection, shallow and deep geoelectrical tomography surveys as well as passive seismic surveys, including single-station measurements and 2D arrays, were performed. These investigations aimed to support the development of a subsurface geological model of the study area for seismic microzonation. This paper presents and discusses the preliminary results of a Deep Electrical Resistivity Tomography (DERT) survey, reaching an investigation depth of approximately 2 km. Campi Flegrei, located west of Naples, is one of the most active and extensively studied volcanic areas in the world. It is a large caldera formed by massive explosive eruptions that occurred thousands of years ago. In recent decades, the area has been affected by intensified seismic activity and bradyseism, expressed as ground uplift and subsidence driven by subsurface magmatic processes. Several geological and volcanological aspects of the Campi Flegrei caldera are still debated within the scientific community, and many questions remain open regarding the magmatic systems responsible for caldera-forming eruptions. A single, widely accepted model has yet to emerge; however, ongoing and newly proposed investigations continue to improve our understanding of the dynamics of the Campi Flegrei caldera. In this framework, shallow and deep Electrical Resistivity Tomography were carried out in order to obtain the electrical resistivity distribution associated with volcanic features, such as hydrothermal systems, fluid interactions and temperature variations (Finizzola et al., 2006). The acquired DERT data set was processed and elaborated through a procedure built ad hoc for this type of geoelectric surveys (Rizzo et al., 2004) and an optimization of the field work was used to overcome the logistical difficulties of the area (heavy urbanisation, traffic, restricted traffic area, etc.). All the data acquired was appropriately processed (Rizzo et al., 2022) to obtain a 3D model of the subsoil resistivity, providing useful information on the subsoil of the Campi Flegrei volcanic area.

 

References

Finizola, A. Revil, E. Rizzo, S. Piscitelli, T. Ricci, J. Morin, B. Angeletti, L. Mocochain, and F. Sortino (2006). Hydrogeological insights at Stromboli volcano (Italy) from geoelectrical, temperature, and CO2 soil degassing investigations. Geophysical Research Letters, vol. 33, l17304, 2006

Rizzo E., Colella, A., Lapenna, V. and Piscitelli, S. (2004). “High-resolution images of the fault controlled High Agri Valley basin (Southern Italy) with deep and shallow Electrical Resistivity Tomographies”. Physics and Chemistry of the Earth, 29, 321-327

Rizzo E., V. Giampaolo, L. Capozzoli, G. De Martino, G., Romano, A. Santilano, A. Manzella (2022). 3D deep geoelectrical exploration in the Larderello geothermal sites (Italy), Physics of the Earth and Planetary Interiors, volume 329-330, 106906 doi: https://doi.org/10.1016/j.pepi.2022.106906

How to cite: Rizzo, E., Piscitelli, S., Stigliano, F., and Lapenna, V. and the Working group MS-Campi Flegrei project of CNR (IGAG-IMAA): Deep Electrical Resistivity Tomography (DERT) in the Campi Flegrei area (Naples, Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4950, https://doi.org/10.5194/egusphere-egu26-4950, 2026.

EGU26-5504 | Orals | GI5.1

Application of geoelectrical methods in environmental and engineering geophysics 

Andre Revil, Ahmad Ghorbani, Feras Abdulsamad, Julia Holzhauer, Olivier Plé, Pierre-Allain Duvillard, Pierre Vaudelet, and Pierre Dick

In this presentation, we will discuss the increasingly important role of electrical resistivity, induced polarization and self-potential tomography in engineering geophysics and the development of joint approaches that can be applied to image water content, permeability, and water flow at various scales. We will first focus on applications to dams and landslides to demonstrate the usefulness of these methods to locate leaks and get a better understanding of the role of ground water flow in clay-rich landslides and mudflow. Then, we will show case a new model of induced polarization that can be applied to cement and concrete and based on fractal theory. Induced polarization can be used as a non-intrusive and non-destructive technique to image and monitor the evolution of cementitious materials, with the objective of retrieving their water content and hydration state. We will show the performance of the model using a collection of cement paste samples (CEMI and CEMV) and corresponding mortar samples (MORI and MORV), all cured for 60 days, with water-to-cement (w/c) ratios ranging from 0.35 to 0.60. Spectral induced polarization measurements are performed in the frequency range 10 mHz-45 kHz. For the cement pastes, both the in-phase conductivity and the magnitude of the quadrature conductivity increase systematically with increase of the w/c (water-to-cement) ratio. The electrical properties of the mortars scale proportionally with those of the corresponding cement pastes, and the proportionality coefficient can be predicted from the volume fraction of cement. The complex conductivity data are well-fitted by a double Cole Cole model, and the normalized chargeability is found to be proportional to the quadrature conductivity, consistent with theoretical expectations. The experimental data are explained using a dynamic Stern layer model associated with the polarization of the inner component of the double layer coating the surface of the C-S-H minerals. Experiments are also performed to monitor the hydration phase of cement pastes like CEMI. To our knowledge, this is the first mechanistic-based interpretation of the complex conductivity spectra of cement pastes and mortars. These results open new perspectives for non-invasive monitoring of concrete in civil and nuclear engineering applications. We will show some time-lapse tomograms obtained inside the PALLAS project demonstrating this point. Furthermore, we will discuss also some applications to raw earth materials for building construction and how we can use time-lapse tomography to image their water content over time.

How to cite: Revil, A., Ghorbani, A., Abdulsamad, F., Holzhauer, J., Plé, O., Duvillard, P.-A., Vaudelet, P., and Dick, P.: Application of geoelectrical methods in environmental and engineering geophysics, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5504, https://doi.org/10.5194/egusphere-egu26-5504, 2026.

EGU26-6403 | Posters on site | GI5.1

High-Resolution Multichannel Analysis of Surface Waves (MASW) Imaging of Karst Features in Carbonate Environments of Eastern Saudi Arabia 

Tanzeel Ur Rehman Sabir, Nordiana Binti Mohd Muztaza, and Khan Zaib Jadoon

Carbonate terrains of the Eastern Province of Saudi Arabia are highly susceptible to subsurface hazards due to intense weathering, fracturing, and karstification. Features such as dissolution cavities, weakened zones, and fault-related discontinuities pose significant risks to infrastructure in a region experiencing rapid urban and industrial development. Accurate and non-invasive characterization of these concealed features is therefore critical for geotechnical risk mitigation.

This study investigates the effectiveness of the Multichannel Analysis of Surface Waves (MASW) technique for identifying and characterizing karst features and fault zones in complex carbonate environments. MASW utilizes the dispersive behavior of Rayleigh waves to derive shear-wave velocity (Vs) profiles, which are sensitive to variations in material stiffness, fracturing, and void development. These velocity contrasts provide valuable indicators of subsurface heterogeneity associated with karst and structural deformation.

Field investigations were conducted at representative sites exhibiting varying degrees of carbonate weathering and karst development. Prior to full-scale data acquisition, parameter sensitivity analysis is performed to optimize survey design, including geophone spacing, spread length, source offset, and sampling interval. MASW data were processed through dispersion analysis and inversion to generate detailed Vs profiles and lateral velocity variations. Anomalous low-velocity zones and abrupt velocity gradients are interpreted as indicators of cavities, fractured layers, and fault zones. The results demonstrated that MASW provides reliable, high-resolution subsurface characterization in karst-prone carbonate terrains, offering a cost-effective and non-invasive tool for identifying geotechnical hazard zones and supporting safer infrastructure planning.

How to cite: Sabir, T. U. R., Mohd Muztaza, N. B., and Jadoon, K. Z.: High-Resolution Multichannel Analysis of Surface Waves (MASW) Imaging of Karst Features in Carbonate Environments of Eastern Saudi Arabia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6403, https://doi.org/10.5194/egusphere-egu26-6403, 2026.

EGU26-7452 | Orals | GI5.1

Imlaymed: a freeware software for the GPR imaging of stratified soils 

Giuseppe Esposito, Fabio Capparelli, Ilaria Catapano, Luigi Capozzoli, Gregory De Martino, Gianfranco Morelli, Ding Yang, and Raffaele Persico

In some cases, soils exhibit a layered structure clearly identified even at the depth scales investigated by Ground Penetrating Radar (GPR) surveys. However, not many methods and computational tools are available that systematically address imaging in layered soils. Imlaymed (Imaging in Layered Media) is a Python graphical user interface (GUI) freeware software specifically designed to tackle this problem. The code assumes either a two layered soil or a cavity embedded within a homogeneous soil. In the latter case, the cavity is locally interpreted as a three-layered medium. The interfaces between adjacent layers are assumed smooth—which is geologically reasonable—although not necessarily planar. However, the non-flatness of the layers precludes the possibility of obtaining an analytical solution. Consequently, Imlaymed addresses the focusing and time–depth conversion issues as an imaging problem rather than an inverse scattering problem. The method explicitly accounts for the presence of two distinct propagation velocities within the soil, which results in geometric distortions, including dilation and compression effects on both the targets and the distances among them. Imlaymed aims to mitigate these distortions. The current release represents an initial version of the software, to be progressively updated and extended. Future developments are expected to introduce additional capabilities—e.g. time-reverse migration—and to enhance the existing features, e.g. through the incorporation of AI techniques and the optional use of parallel computing. In particular, Imlaymed will aid to generation of slices directly in the spatial domain instead of the common slices built up in time domain.

The methodology underlying the code is based on our previous results [1-6]. The implementation of this code has improved both the computational efficiency and the ease of use of the algorithms. Notwithstanding, the user of Imlaymed is supposed to have some non-too-basic background experience in GPR prospecting.

Imlaymed is distributed under AUL/ANCL License (Academic Use License/Academic Non-Commercial License).

Acknowledgements

This work has been implemented within the activities of the Research Project “Georadar e avanzamento delle investigazioni: un’applicazione economica alla sicurezza stradale”, financed by University of Calabria.

References

  • Persico, G. Morelli, Combined Migrations and Time-Depth Conversions in GPR Prospecting: Application to Reinforced Concrete, Remote Sens. 2020, Volume 12, Issue 17, 2778, open access, DOI 10.3390/rs12172778.
  • Persico et al. “A posteriori insertion of information for focusing and time–depth conversion of ground-penetrating radar data”, Geophysical Prospecting, open access, https://doi.org/10.1111/1365-2478.13369, 2023.
  • Persico et al., ­GPR mapping of cavity in complex scenarios with a combined time-depth conversion, Sensors, MDPI, Sensors 2024, 24(10), 3238; https://doi.org/10.3390/s24103238, 2024.
  • Persico et al., An innovative time-depth conversion for the management of buried scenarios with strong discontinuities, Journal of Applied Geophysics vol. 227, 105435, DOI 10.1016/j.jappgeo.2024.105435, 2024.
  • Yang et al., Accounting for the Different Propagation Velocities for the Focusing and Time–Depth Conversion in a Layered Medium, Applied Sciences 14(24):11812, 2024.
  • Persico et al., Retrieving the propagation velocity of the electromagnetic waves in a two-layered medium through the diffraction curves, Near Surface Geophysics, 1–13. https://doi.org/10.1002/nsg.70028, 2025.

How to cite: Esposito, G., Capparelli, F., Catapano, I., Capozzoli, L., De Martino, G., Morelli, G., Yang, D., and Persico, R.: Imlaymed: a freeware software for the GPR imaging of stratified soils, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7452, https://doi.org/10.5194/egusphere-egu26-7452, 2026.

EGU26-10509 | Posters on site | GI5.1

Electrical Resistivity Tomography and Ground Penetrating Radar for Bridges: Preliminary Findings from the EMILI Project 

Luigi Capozzoli, Ilaria Catapano, Giovanni Ludeno, Giuseppe Esposito, Gianluca Gennarelli, Carlo Noviello, Francesco Soldovieri, Gregory De Martino, Davide Di Gennaro, Gerardo Romano, Valeria Giampaolo, Angela Perrone, Vincenzo Lapenna, Chiara Ormando, Antonio Di Pietro, Maurizio Pollino, Giacomo Buffarini, Alessandro Lipari, Paolo Clemente, and Alessandro Giocoli

Transportation networks rely heavily on bridges whose safe operation depends on maintaining structural soundness. Natural phenomena, such as landslides and human-induced incidents, pose significant threats to bridges, with consequences ranging from compromised safety to complete failure and service interruption. Multiple variables determine the extent of structural deterioration, including the nature of hazardous events, material composition, and existing maintenance conditions. A comprehensive evaluation of landslide-related threats necessitates examining a variety of factors, including the geophysical properties of the subsoil and an in-depth knowledge of the bridge key structural elements, such as its foundations, piers, and abutments, as well as their current state of conservation.

Supported by the FABRE consortium, the EMILI project - ElectroMagnetic techniques for Investigating Landslide and structural damages due to their Impacts on bridges - aims to establish uniform protocols and operational frameworks for electromagnetic investigation techniques in bridge-landslide hazard evaluation. By targeting Electrical Resistivity Tomography (ERT) and Ground Penetrating Radar (GPR), EMILI advances the standardization, reliability, and field implementation of electromagnetic approaches.

Initial findings from EMILI are discussed here, encompassing two primary contributions. The first concerns a comprehensive literature analysis examining both capabilities and constraints of ERT and GPR in field applications involving bridges, landslides, and their interactions. The second deals with preliminary results from simplified numerical models exploring the detection potential of ERT and GPR when applied via conventional and unconventional measurement configurations. Specifically, surface and borehole data from simulated scenarios involving diverse lithologies, foundations, and water content are considered and processed to establish the potential and limitations of ERT and GPR in estimating the shape and depth of the foundation piles.

Preliminary synthetic results are promising and demonstrate the capability of ERT and GPR to identify foundation structures in simplified geological contexts.

How to cite: Capozzoli, L., Catapano, I., Ludeno, G., Esposito, G., Gennarelli, G., Noviello, C., Soldovieri, F., De Martino, G., Di Gennaro, D., Romano, G., Giampaolo, V., Perrone, A., Lapenna, V., Ormando, C., Di Pietro, A., Pollino, M., Buffarini, G., Lipari, A., Clemente, P., and Giocoli, A.: Electrical Resistivity Tomography and Ground Penetrating Radar for Bridges: Preliminary Findings from the EMILI Project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10509, https://doi.org/10.5194/egusphere-egu26-10509, 2026.

EGU26-11446 | Orals | GI5.1

Integrated geophysical and participative approaches for geothermal resources evaluation in urban areas in Southern Italy 

Valeria Giampaolo, Vincenzo Serlenga, Marianna Balasco, Gregory De Martino, Angela Perrone, Tony Alfredo Stabile, Vincenzo Lapenna, Ferdinando Napolitano, Enzo Rizzo, Serena Panebianco, Luigi Martino, Paolo Capuano, Massimo Blasone, Davide Bubbico, Valentina Cataldo, and Ortensia Amoroso

This work is supported by the projects TOGETHER – Sustainable geothermal energy for two Southern Italy regions: geophysical resource evaluation and public awareness (https://www.together-prin.it/) and ITINERIS – Italian Integrated Environmental Research Infrastructures System (https://itineris.cnr.it/), funded by the European Union – Next Generation EU (PNRR, M4C2, Investments 1.1 and 3.1, respectively).

As part of the ITINERIS project, the geophysical laboratory of CNR-IMAA was upgraded with advanced geophysical instrumentation characterized by lower operational costs, increased flexibility, higher sensitivity, and faster acquisition rates. The availability of dense and flexibly deployable geophysical sensors significantly improves survey resolution, particularly in complex urban and semi-urban environments, thereby supporting sustainable and resilient urban development.

Under the TOGETHER project, the upgraded instrumentation was tested at pilot sites, including the Sele River Valley (SRV) in the Campania region (Southern Italy). This area hosts numerous thermal springs and wells with temperatures reaching up to 48 °C, currently used for spa and therapeutic purposes. These characteristics make the SRV a natural laboratory for testing integrated geophysical approaches aimed at identifying geothermal targets in proximity to existing communities and infrastructure.

Geothermal energy, particularly low- to medium-enthalpy systems, represents a key renewable resource for the energy transition, enabling the sustainable exploitation of local resources, the reduction of greenhouse gas emissions, and the strengthening of regional energy resilience. Integrated geophysical investigations play a crucial role in reducing exploration uncertainty and promoting environmentally responsible geothermal development.

In the SRV area, geophysical surveys were conducted over a target zone of approximately 6 × 8 km², centered on the hottest thermal manifestations. A comprehensive geophysical dataset was successfully acquired in a challenging urban and semi-urban context characterized by logistical constraints and high levels of anthropogenic noise. Multi-scale and multi-resolution three-dimensional subsurface electrical resistivity models were derived using shallow and deep Electrical Resistivity Tomography (ERT/DERT) and Magnetotelluric (MT) surveys. In parallel, ambient seismic noise recordings were acquired and processed using single-station HVSR analyses and array-based Ambient Noise Tomography (ANT).

In parallel with fieldwork, public engagement activities were implemented to foster trust and collaboration with local stakeholders. These activities included the involvement of high school students and teachers, communication through municipal social media channels, the distribution of participation certificates, and the organization of a final dissemination event aimed at citizens, local institutions, schools, and stakeholders. The event was dedicated to sharing the results and research activities developed in the area as part of the TOGETHER project, with a particular focus on energy sustainability and the enhancement of local geothermal resources, also through direct dialogue between researchers and the public. These initiatives proved essential for ensuring transparency, site accessibility, and awareness of local geothermal potential.

The results demonstrate the feasibility and effectiveness of an integrated geophysical and participatory approach, highlighting the importance of public engagement and standardized workflows for sensor deployment and data processing.

How to cite: Giampaolo, V., Serlenga, V., Balasco, M., De Martino, G., Perrone, A., Stabile, T. A., Lapenna, V., Napolitano, F., Rizzo, E., Panebianco, S., Martino, L., Capuano, P., Blasone, M., Bubbico, D., Cataldo, V., and Amoroso, O.: Integrated geophysical and participative approaches for geothermal resources evaluation in urban areas in Southern Italy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11446, https://doi.org/10.5194/egusphere-egu26-11446, 2026.

EGU26-17896 | Posters on site | GI5.1

Using surface-NMR measurements to study the effects of compaction measures on the properties of lignite mining dumps 

Thomas Hiller, Stephan Costabel, Gundula Erdmann, and Elisabeth Schönfeldt

In the last 15 to 20 years, a sudden spike of liquefaction events after groundwater rebound on inner dumps in the Lusatian mining district resulted in around 30,000 hectares of land being closed to public access. One of the common modern compaction methods used is the gentle-blast-compaction (GBC), in which minimal explosive charges are placed in defined depth horizons (below the groundwater table) and detonated one after the other from the bottom upwards. The primary objective is to improve the ground stability by locally collapsing the pore structure of the material. This increases the bulk density of the dump material and reduces the air and waterfilled proportion of the pore space. Usually, direct geotechnical methods like drillings or cone penetration tests (CPT) are used to verify successful compaction. Within the “VerLaUf” project, we investigate the suitability of various airborne and ground-based geophysical methods for the non-invasive evaluation of these compaction measures. In the present study, we focus in particular on the applicability of two electromagnetic methods, transient electromagnetics (TEM) and surface nuclear magnetic resonance (SNMR). The TEM measurements are used to obtain a resistivity model of the subsurface which is needed for the inversion and interpretation of the SNMR data. Due to the direct correlation between SNMR signal amplitude and water content (porosity) as well as SNMR relaxation time and pore size, the SNMR method promises not only qualitative but also quantitative results about the change in the (water-filled) pore space after GBC.

Field campaigns were carried out over the course of three years, where the GBC took place after the first measurement campaign at depths ranging from 7 m to 32 m. The subsequent measurement campaigns were carried out after the GBC, with waiting times of approx. five and 15 months, respectively. The TEM and SNMR measurements consisted of 1D soundings along a 2D profile which was about 450 m long. One reference point, without GBC and about 400 m away from the profile, was measured for comparison and to identify seasonal variations in the data. All measurements were carried out with identical field setups and measurement parameters (loop size, number of averaging measurement repetitions, etc.). The recorded data were processed in an identical manner and a QT-inversion was used to derive a depth resolved partial water content model, i.e., the water content as function of depth and relaxation time. Due to the noisiness of the SNMR data, we used a permeability index, a combination of SNMR signal amplitude and relaxation time, to evaluate the results. By doing so, we reduce the inherent ambiguity (especially in noisy data) between the two parameters. Comparing the results from the first with the last field campaign shows, that a reduction of the permeability index within the GBC targeted layers of about 33 percent is detected, which is indicative for a respective compaction.



How to cite: Hiller, T., Costabel, S., Erdmann, G., and Schönfeldt, E.: Using surface-NMR measurements to study the effects of compaction measures on the properties of lignite mining dumps, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17896, https://doi.org/10.5194/egusphere-egu26-17896, 2026.

EGU26-18388 | Orals | GI5.1

Surface-to-Bedrock Imaging of the Sakarya Basin Based on Integrated Analysis of Ambient Noise and Seismic Data 

Ali Silahtar, Mustafa Şenkaya, Hasan Karaaslan, and Emrah Budakoğlu

Recent earthquakes in Türkiye, including the 2020 Samos and 2023 Kahramanmaraş events, have once again underscored the significant impact of local ground conditions and the three-dimensional structure of alluvial basins on earthquake ground motion. In such settings, seismic wave propagation is strongly controlled by basin geometry, sediment thickness, and shear-wave velocity (Vs) contrasts, which can significantly affect ground motion characteristics and increase uncertainties in seismic hazard assessments. For this reason, generating reliable and spatially detailed Vs models at the basin scale has become increasingly important.

The Sakarya Basin, located within the active tectonic framework of the North Anatolian Fault Zone, represents a suitable case study due to its young alluvial deposits and high seismic potential. In this study, the shear-wave velocity structure of the basin is investigated from the surface down to the engineering bedrock through an integrated analysis of ambient noise and seismic data, combining both active and passive seismic methods. Field investigations comprise 533 MASW and ReMi measurements, including 316 newly acquired sites, providing dense coverage of the shallow subsurface. To constrain deeper velocity structures, ambient noise array recordings collected at 61 locations were analyzed using the Spatial Autocorrelation (SPAC) method. The resulting one-dimensional Vs profiles were interpreted together with existing geological and geophysical information and integrated within a GIS-based framework to construct a coherent surface-to-bedrock shear-wave velocity model of the Sakarya Basin.

The resulting model reveals extensive low-velocity sedimentary zones that can delay seismic wave propagation and lead to ground motion amplification within specific frequency ranges. These observations improve the understanding of basin-related site effects and support the identification of areas that may be more vulnerable to seismic amplification. The main contribution of this study lies in the basin-scale integration of high-density active seismic measurements with SPAC-derived ambient noise data, enabling surface-to-bedrock imaging with a level of spatial resolution not previously available for the Sakarya Basin. The resulting Vs model provides an improved representation of both shallow and deep subsurface conditions, offering valuable insights for site classification and basin-related ground motion studies. This research was conducted within the scope of the TÜBİTAK-funded project no. 124Y188.

How to cite: Silahtar, A., Şenkaya, M., Karaaslan, H., and Budakoğlu, E.: Surface-to-Bedrock Imaging of the Sakarya Basin Based on Integrated Analysis of Ambient Noise and Seismic Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18388, https://doi.org/10.5194/egusphere-egu26-18388, 2026.

EGU26-21428 | Posters on site | GI5.1

Near-surface geophysics for characterizing complex subsurface settings in historically layered monumental urban areas 

Giuseppe Calamita, Luigi Capozzoli, Gregory De Martino, Jessica Bellanova, Sabatino Piscitelli, Angela Perrone, Luigi Martino, and Maria Gallipoli

Historical urban centres of high cultural and monumental relevance are commonly characterized by complex and highly heterogeneous subsurface settings, resulting from the superposition of natural geological deposits, archaeological layers, and centuries of anthropogenic modifications. In such contexts, limited or fragmented subsurface knowledge may hinder archaeological interpretation and constrain multidisciplinary analyses aimed at urban reconstruction and heritage preservation.

This contribution is framed within the Italian PRIN 2022 project NEW AGE (New Integrated Approach for Seismic Protection and Enhancement of Heritage Buildings on Historic Earthen Deposits) and presents results from non-invasive geophysical investigations conducted at two emblematic monumental sites: the Roman Amphitheatre (Arena) of Verona and the Santa Sofia monumental complex in Benevento, both characterized by prolonged and stratified occupation histories, leading to highly heterogeneous near-surface conditions. The investigations benefited from advanced geophysical instrumentation made available through the IRPAC and ITINERIS research infrastructure (funded through regional and national programs, respectively), supporting enhanced data acquisition capabilities within the project framework.

We propose a multi-scale, multi-method geophysical approach designed to improve the characterization of shallow subsurface conditions in densely built and historically layered urban environments. The investigation strategy combines ground-penetrating radar (GPR), electrical resistivity tomography (ERT), and seismic methods, selected to explore complementary physical properties and depth ranges while accommodating site-specific logistical and conservation constraints.

GPR surveys provided high-resolution imaging of shallow subsurface heterogeneities and anthropogenic features, supporting the identification of archaeological remains and spatial variations within near-surface layers. ERT investigations complemented these results by resolving broader geological structures and deeper resistivity contrasts, allowing reconstruction of subsurface variability at different spatial scales. Seismic measurements contributed additional constraints on subsurface layering and mechanical properties.

The combined interpretation of the different datasets acquired, supported by archaeological and geotechnical information where available, provides a robust and physically consistent reconstruction of the shallow subsurface in complex, historically layered monumental settings. The multi-method geophysical framework enables the identification of stratigraphic heterogeneities, anthropogenic layers, and buried structures, reducing subsurface uncertainty in complex heritage contexts and supporting subsequent geological, archaeological, and engineering analyses.

How to cite: Calamita, G., Capozzoli, L., De Martino, G., Bellanova, J., Piscitelli, S., Perrone, A., Martino, L., and Gallipoli, M.: Near-surface geophysics for characterizing complex subsurface settings in historically layered monumental urban areas, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21428, https://doi.org/10.5194/egusphere-egu26-21428, 2026.

EGU26-21551 | ECS | Orals | GI5.1

Integrated Passive and Active Seismic Methods for Subsurface Characterization of the Campi Flegrei area (Southern Italy) 

Silvia Giallini, Maurizio Simionato, Maria Grazia Caielli, Stefano Catalano, Federica Davani, Roberto de Franco, Iolanda Gaudiosi, Gabriele Fiorentino, Marco Mancini, Attilio Porchia, Federica Polpetta, Francesco Stigliano, Emanuela Tempesta, Daniel Tentori, and Giuseppe Tortorici

Active volcanic areas located within densely urbanized regions require reliable geophysical methods to characterize the subsurface and support seismic hazard assessment and monitoring strategies. The Campi Flegrei area (Southern Italy) represents a paradigmatic example, where hydrothermal activity, fluid circulation, and strong lateral heterogeneities, combined with urban constraints, make subsurface velocity modeling particularly challenging.

In this framework, and in response to the seismic sequence that began in 2023, an extensive campaign of experimental geophysical investigations was promoted and funded by the Italian Department of Civil Protection in the Campi Flegrei area. We present a multi-method seismic investigation based on 66 Horizontal-to-Vertical Spectral Ratio (HVSR), 11 2D seismic array and 20 Multichannel Analysis of Surface Waves (MASW) measurements at 20 sites. Shear-wave velocity (Vs) profiles were derived at each site through joint inversion of the dispersion curve (retrieved from 2D seismic array data and MASW) with ellipticity of the Rayleigh waves.

All HVSR measurements consistently exhibit a low-frequency peak (f0 ≈ 0.2–0.5 Hz), interpreted as the response of the deep caldera fill sediments.  Further peaks at frequencies above 0.5 Hz may be associated with shallow impedance contrasts. The fundamental frequency (f0) seems reflecting lateral variations in the depth and stiffness of the caldera fill. Significant variability in HVSR amplitude, sharpness and polarization, reflects the interplay between geological heterogeneity and urban noise sources.

The joint inversion approach reduces model non-uniqueness and provides well-constrained Vs profiles, improving the physical interpretation of HVSR features in terms of stratigraphy and velocity contrasts. This study highlights the potential of HVSR-based methods in active volcanic and urbanized settings and emphasizes the importance of combining passive and active methods to address geological complexity and anthropogenic interference, paving the way for further multi-scale studies and their application in urban volcanic contexts worldwide.

The resulting Vs velocity profiles provide further information for interpreting the stratigraphic features and discontinuities of the caldera fill, useful for integration with other type of studies (hydrothermal alteration) and other type of geophysical data

Moreover, the results of this study offer valuable tools for geohazard assessment and constitute a preliminary step towards the seismic microzonation of the area.

How to cite: Giallini, S., Simionato, M., Caielli, M. G., Catalano, S., Davani, F., de Franco, R., Gaudiosi, I., Fiorentino, G., Mancini, M., Porchia, A., Polpetta, F., Stigliano, F., Tempesta, E., Tentori, D., and Tortorici, G.: Integrated Passive and Active Seismic Methods for Subsurface Characterization of the Campi Flegrei area (Southern Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21551, https://doi.org/10.5194/egusphere-egu26-21551, 2026.

EGU26-21992 | Orals | GI5.1

Rapid Microgravity Assessment of Subsurface Cavities Using Terrain-UnCorrelated Anomalies 

Maurizio Milano, Giovanni Florio, Giuseppe Ferrara, Federico Cella, and Lorenzo Ricciardi

In emergency engineering contexts, conventional gravity-processing workflows based on Bouguer anomaly computation are often impractical, as they require high-resolution digital elevation models and assumptions about terrain density, both of which introduce delays and additional uncertainty.

Following a localized collapse beneath track 2 at the EAV Pozzuoli railway station (Naples, Italy), a microgravity survey was conducted to support rapid subsurface characterization. Optical inspections indicate that the cavity extends approximately 4.5 m deep and 6 × 6 m, and affected both tracks, and caused visible settlement of the station platforms. The objectives of the gravity investigation are to assess (i) the spatial relationship between the detected cavity and the pedestrian underpass connecting the station building to platform 2, and (ii) the downstream path of wastewater.

In this study, we adopt a fast gravity data processing strategy to estimate the gravity component generated by lateral subsurface density contrasts (Florio et al., 2025). A linear regression between Free-Air Anomalies and elevation enables a parameter-free decomposition of the gravity field into a terrain-correlated component (TCA) and a terrain-uncorrelated component (TUCA). This approach enhances the detection of anomalous features such as cavities or mass deficits and allows for the independent estimation of average terrain density.

TUCA processing is rapid, requires minimal input data, and can be performed directly in the field, making it particularly suitable for preliminary evaluations in time-critical geotechnical settings. This paper presents the TUCA workflow and its application to the Pozzuoli railway station case study, including the survey design and key results.

How to cite: Milano, M., Florio, G., Ferrara, G., Cella, F., and Ricciardi, L.: Rapid Microgravity Assessment of Subsurface Cavities Using Terrain-UnCorrelated Anomalies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21992, https://doi.org/10.5194/egusphere-egu26-21992, 2026.

EGU26-1537 | ECS | Posters on site | GI5.2

Study on automated detection methods of shallow surface soil water content based on GPR signal level 

Yunfeng Fang, Tao Ma, Zheng Tong, and Siqi Wang

This paper addresses automated, uncertainty-aware estimation of shallow surface soil water content (SWC) from ground-penetrating radar (GPR) at the A-scan signal level, overcoming the reliance of conventional workflows on manually picked interfaces and empirical dielectric–moisture curves. Refined gradient soil boxes of sandy and clayey soils (0–30 % gravimetric SWC in 1 % steps) are constructed, 2 GHz GPR and TDR permittivity data are acquired, an effective time window is defined by consistency between travel-time inferred permittivity and TDR, and three physically interpretable attributes—time delay, envelope amplitude area (AEA) and centroid frequency (CF)—are extracted as candidate predictors. Attribute analysis reveals that AEA and CF behave as global indicators that are highly sensitive to SWC in sandy soil, whereas the local delay feature responds more strongly and monotonically in clayey soil because of its higher specific surface area, stronger bound-water effects and slower saturation. Single-indicator regressions already achieve high coefficients of determination (R² up to 0.98 for delay in sand and not less than 0.80 for the remaining indicators), but also expose soil-dependent bias and instability. To exploit the complementary information content of the three attributes, a three-indicator SWC model is built whose weights are obtained by multiplicatively fusing random forest importance with grey relational degree, thereby balancing direct predictive power with dynamic trend consistency. Model comparison shows that, for sandy soil, the three-indicator formulation reduces mean squared error (MSE) by more than 80 % relative to AEA- or CF-only models and remains comparable to delay-only regression, while for clayey soil it lowers MSE by approximately 27 %, 30 % and 51 % with respect to delay-, CF- and AEA-based models, respectively. Bayesian linear and nonlinear regression, combined with Monte Carlo sampling, is further employed to infer posterior distributions of model parameters and observation noise. The resulting credible intervals demonstrate that both model and data uncertainties remain within controllable ranges across the calibrated three-indicator space, with delay exhibiting particularly high predictive reliability. Building on the near-consistent predictions of the delay-only and three-indicator models, an error-recursive optimisation framework is proposed for fully automated SWC inversion. For each A-scan, an initial SWC is assumed, mapped to a travel time via the delay model, and used to recompute AEA and CF within the corresponding time gate; the discrepancy between the two SWC estimates is iteratively minimised until a strict convergence criterion is satisfied. The framework is implemented in dedicated software and validated on independent gradient-box samples and a 1.6 m field transect, where GPR-derived SWC profiles agree well with TDR yet avoid the low-moisture underestimation and high-moisture overestimation characteristic of TDR plus Topp/Roth mixing models. In terms of practical performance, the automated scheme markedly reduces manual interaction, maintains smooth SWC gradients even under 3 % step changes, and remains robust to mixing-induced heterogeneity in clayey samples. Overall, the study demonstrates a technically rigorous pathway toward highly automated, high-resolution GPR monitoring of shallow SWC with explicit quantification of predictive uncertainty.

How to cite: Fang, Y., Ma, T., Tong, Z., and Wang, S.: Study on automated detection methods of shallow surface soil water content based on GPR signal level, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1537, https://doi.org/10.5194/egusphere-egu26-1537, 2026.

Lake-Cuitzeo: Dual-Impact Stratigraphy; Cueva da Pedra-Pintada: Dual-Comet Celestial-Cartography.

Brazilian Pedra-Pintada site´s lowest stratum provided 14C and luminescence dates for End-Pleistocene, pre-pottery, Paleoindian middens, with soft sand, charcoal and red pigment layer. That same pigment, chemically identified, was used in cave-wall pictograms above, providing stratigraphic dating (Roosevelt,1996; Michab,1998). These pictograms, in celestial-paleo-cartography, depict two comets (Bujatti-Narbeshuber,1997a).

That lowest, dated, Pedra-Pintada stratigraphic-layer of 30 cm, associated with two comet-pictograms, is most tellingly followed by culturally sterile 30 cm soil, again finally followed by Holocene-middens (65 cm) of thriving pottery-age populations.

The anthropomorphic pictograms encode the concentric comet-nucleus-coma-halo threefold structure as descending head identically consisting of three concentric layers, only one with radiant hair. Dual comet-dust and plasma-tail is encoded as parallel legs extending upwards. Two different comet-stages and two different comet-trajectories are evident: one with concentric comet-head, radiant hair, descending, the other comet-head, without hair, not radiating, burnt out, as concentric impact-crater “fallen-dead”, with parallel legs, tied together, also forming “H”= ”fallen-dead”-symbol.

Magdalenian Impact Sequelae Symbolizations (MISS) by AO-KISS-impact-survivors in Göbelli-Tepe use “H” on T-pillars 43 and 18. The “SNAKES-((H-I-T))-SPOT” decoding formula means: (Prof.Klaus) Schmidt-Never-Assumed-KISS-Equates-Snakes (= Taurid impactors), that “H”= “Hurt” the  “I”= “Intact-upright-alive”C “T”-pillar. “Hurt-fallen-dead” symbolization by “I”-column=T-pillar-symbol of ritual-centers-Mid-Atlantic-Plateau-MAP-Civilization, cartographic 90° (“I”=West-up to North-up=”H” ) Solar-Polar-Orientation-Transition, within two-step Mega-tsunami = ((double-brackets)). This abstract-composite-proto-writing symbolizes AO-KISS induced two-step Mid Atlantic Ridge & Plateau Lowering Events (MARPLES) within T-pillar-43-celestial-paleo-cartography (Bujatti-Narbeshuber,2022), precession dated 12.850-13.000 cal BP (Sweatman,2017, 2022).

Pedra-Pintada, dual-comet, pictogram-stratigraphy 14C dated 11.145 + - 135, calibrated to 13.300- 12.750 cal BP (95% confidence level) has mean calibrated age 13,010 cal BP. This fits AO-KISS-Bipolar-Sulfate-Impact-Volcanism-Heptaplet-proxi Laacher-See-Tephra isochrone of 13,006 + - 9 cal BP (Bujatti-Narbeshuber,1997a,Reinig,2021). It also fits earliest Mayan Codex Troano calendar date 13,124 cal BP and maximally 274 years later Continental-Ice (CI)-Carolina-Bays-KISS date 12.850 cal BP.

Dual CI-AO-KISS-MARPLES fit Mexican-Lake-Cuitzeo (MLC) stratigraphy consisting of three-layered-lacustrine “Black-White-Graphite-Mats”.

There 14C-“Dead-Old-Graphite” (DOG-)-Mats” mark P/H-boundary-AO-KISS-MARPLES with Impact-Catastrophic-Climate-Transition (ICCT):

 

 

MLC-stratigraphy-level below (2,55 m) confirms by “Black-Mats” from high humidity algal organic carbon, identity with North American “Black-Mats”, following from Continental-Ice-KISS with secondary meteoritic-ice-ejecta-impacts, shaping 500.000 mathematical ellipses, Carolina-Bays, into earlier AO-KISS-“White Mats” (Muck,1976;Davias,2007;Zamora,2015;Bujatti-Narbeshuber,2023).

MLC-stratigraphy-level above (2,70 m) confirms by “White-Mats” identity with North American precursor of Carolina-Bay-formation as bleached-sand A2-horizon, non-fossiliferous-sand Goldsboro-Ridge-Enigma, nearly pure silicate, industrial white glass-production-grade-sand (Daniels&Gamble,1969,1970,1972), K/Pg-like (Senel,2023), European Usselo Horizon (Andronikov,2016), all documenting aeolian-transport by AO-KISS-MARPLES-Megaplume of ocean-floor-magmatic-volcanic-clastic-material in meso-stratospheric Mega-Hunga-Tonga-(2022)-like steam-plume, raining down in torrential-acidic-bleaching waterfalls (Bujatti-Narbeshuber,2022,2023).  

MLC-lowest-stratigraphy-level with Nano-Diamond-peak (2,75-2,8 m) as 14C-depleted “DOG-Mats". Disturbing MLC-core 14C dating, below “White Mat” (2,75 m), a 1 cm thick layer, that  ”contains thin millimeter-sized-interbeds of black organic carbon…without form or structure” of almost pure elemental carbon, enigmatic, not “plant-derived kerogenous organic-matter”. “Currently, the source of this old carbon remains unclear” (Israde-Alcántara,2012).

Ocean-floor Black-Smokers, producing graphite with very old 14C-ages (Estes, Nature Communications, 2019), should fully account for “DOG-Mats” through AO-KISS-MARPLES-Megaplume aeolian-transport around Azores-Triple-Junction.

(Bujatti-Narbeshuber,1994,1995,1997a,b,2002,2008,2022,2023,2024a,b,c,2025).

How to cite: Bujatti-Narbeshuber, Dr. M.: Pleistocene/Holocene (P/H) boundary oceanic Koefels-comet Impact Series Scenario (KISS) of 12.850 yrs BP Global-warming Threshold Triad (GTT). Part VI, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2154, https://doi.org/10.5194/egusphere-egu26-2154, 2026.

EGU26-3490 | Orals | GI5.2

Assessment of Railway Substructure Integrity using Ground Penetrating Radar 

Christina Plati, Charis Kyriakou, and Andreas Loizos

Railway network is one of the main pillars of modern transport systems, offering safety, energy efficiency and a limited environmental footprint. For this reason, great emphasis should be given on assessing the condition and performance of the railway infrastructure, especially after extreme weather events. Νon-destructive testing offers significant advantages in this context, as it enables continuous inspection without disrupting operation. This study presents the results of a Ground Penetrating Radar (GPR) investigation, carried out on a double-track railway line, following severe flood-related impacts. The aim was to assess the condition of the substructure and identify potential critical locations.

GPR surveys were conducted in both traffic directions using a combination of air-coupled and ground-coupled antennas operating at frequencies of 2.0 GHz, 1.0 GHz, and 400 MHz, allowing detailed characterization of ballast, sub-ballast, and underlying subgrade layers’ thickness. Data acquisition was conducted at operational speeds using a rail-mounted vehicle. The collected raw data were processed using signal enhancement and interpretation techniques, such as filtering, time-zero correction, and stratigraphic analysis. The results were calibrated using available geotechnical information from trial pits and dynamic cone penetration (DCP) tests.

The analysis provided continuous layer thickness estimates at 10 m intervals, revealing both overall structure and local irregularities along the line. While ballast thicknesses were generally consistent (53-59 cm), greater variability was observed in the sub-ballast and subgrade layers, with coefficients of variation exceeding 15-20% in particular sections. Several locations showed abrupt thickness reductions, disrupted stratigraphy, and signal attenuation, and were characterized as potentially critical zones.

The findings confirm that GPR can be effectively used as a non-destructive tool for railway infrastructure assessment, particularly in post-event conditions. The approach supports resilience-oriented asset management by allowing early detection of subsurface anomalies without service disruption and contributing prioritize targeted interventions for sustainable maintenance, and log-term infrastructure safety and performance.

How to cite: Plati, C., Kyriakou, C., and Loizos, A.: Assessment of Railway Substructure Integrity using Ground Penetrating Radar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3490, https://doi.org/10.5194/egusphere-egu26-3490, 2026.

During the curing process of emulsified asphalt cold recycled mixtures (ECRM), mechanical strength gradually develops as internal moisture evaporates. However, the relationship between mechanical property evolution and internal moisture content during the curing of ECRM has not been sufficiently investigated. Moreover, accurate and effective non-destructive methods for monitoring internal moisture loss are still lacking. In this study, low-field nuclear magnetic resonance (LF-NMR) and electrochemical impedance spectroscopy (EIS) were employed as non-destructive techniques to characterize the internal moisture behavior of ECRM with different RAP contents and to analyze its correlation with mechanical performance. LF-NMR testing enables direct characterization of the content, spatial distribution, and migration behavior of internal moisture within a specimen. EIS measures the impedance spectra of materials containing conductive phases. Both techniques offer rapid, non-destructive, and continuous measurement capabilities, allowing visualization of moisture distribution within the material.

The study first evaluated the time-dependent evolution (up to 28 days of curing) of key mechanical properties—including abrasion resistance, Marshall stability, indirect tensile strength (ITS), and splitting tensile modulus (STM)—of ECRM with different RAP contents(0%, 30%, 50%, and 70%). Subsequently, LF-NMR was employed to investigate the content, spatial distribution, and time-dependent migration behavior of free moisture within ECRM containing different RAP contents over a 28-day curing period. The study fabricated working electrodes using epoxy resin and steel rods. The electrodes were buried in the center of ECRM Marshall specimens to measure the electrochemical impedance values of the samples. Given the presence and evolution of internal moisture in ECRM, EIS was then used to monitor the electrical resistance of ECRM with different RAP contents over the same curing period, enabling a quantitative analysis of free moisture evolution. Finally, correlations between the mechanical properties of ECRM and its internal moisture characteristics were established. LF-NMR results indicate that, regardless of RAP content, the internal free moisture in ECRM exhibits a similar distribution pattern: approximately 10% in mesopores (<0.01μm), about 10–30% in intermediate pores (between 0.01μm and 0.1μm), and roughly 60–70% in macropores (>0.1μm). As curing time increases, the internal free moisture in ECRM with different RAP contents consistently migrates from mesopores to intermediate and macropores. This migration behavior results from the combined effects of pore structure characteristics, moisture transport mechanisms, and physicochemical interactions. EIS results showed that impedance increased with curing time, and mechanical performance exhibited a positive correlation with moisture loss. The results demonstrate that LF-NMR and EIS measurements are effective methods for investigating internal moisture characteristics and the evolution of mechanical properties in ECRM. The results reveal the distribution characteristics and migration behavior of internal free moisture in ECRM. These features exhibit a universal pattern and are independent of RAP content.

The findings provide technical guidance for accurately determining the curing time and mechanical strength development of cold-mixed asphalt mixtures. The proposed methods offer significant advantages in non-destructive testing and in situ monitoring. The research conclusions provide a solid foundation for studying the performance of cold-mixed asphalt materials and offer effective solutions for non-destructive testing.

How to cite: Du, H., Zhu, J., Ma, T., Li, R., and Wang, S.: Evolution of Mechanical Properties and Internal Moisture Behavior of Emulsified Asphalt Cold Recycled Mixtures Based on LF-NMR and EIS Non-Destructive Testing Techniques, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3639, https://doi.org/10.5194/egusphere-egu26-3639, 2026.

EGU26-3679 | ECS | Orals | GI5.2

A Noise-Cancellation Pipeline for GPR-Based Asphalt Pavement Compaction Evaluation 

Mingqi Yang, Tao Ma, and Siqi Wang

During asphalt pavement construction, compaction degree is a key indicator of quality control, directly affecting pavement service life and long-term performance. When mounted on a roller, air-coupled ground-penetrating radar (GPR) enables real-time pavement compaction evaluation due to its high efficiency, continuous measurement, and large spatial coverage. However, under practical construction conditions, multiple factors jointly affect the propagation and reflection of electromagnetic waves at the pavement surface. Surface moisture from water sprayed onto roller drums, as well as antenna height variations induced by roller vibration, can cause significant fluctuations in reflection amplitude, thereby reducing the accuracy and stability of GPR-based density predictions.

This study develops a time-domain signal correction framework to improve the accuracy of GPR-based density predictions during pavement compaction. The framework was designed to support automated processing by extracting the pavement surface reflection from full GPR signals and mitigating amplitude distortions induced by construction-related disturbances. Specifically, a semi-blind source separation method based on independent component analysis (ICA) was employed to remove surface moisture–related electromagnetic interference. At the same time, an electromagnetic-empirical model relating antenna height to reflection amplitude was introduced to compensate for vibration-induced variations in antenna height. By jointly accounting for these coupled effects within a unified correction strategy, the proposed framework recovered pavement surface reflections representative of dry conditions at a reference height, thereby enhancing the stability and reliability of GPR-based density estimation.

The proposed framework is validated through FDTD-based numerical simulations and field experiments. The results demonstrate that surface moisture effects and roller-induced antenna height variations can be effectively corrected, whether acting individually or in combination, allowing pavement surface reflection amplitudes to be recovered to a dry state at a standard antenna height. This work provides a practical basis for developing real-time GPR-based pavement compaction evaluation methods under complex construction conditions.

How to cite: Yang, M., Ma, T., and Wang, S.: A Noise-Cancellation Pipeline for GPR-Based Asphalt Pavement Compaction Evaluation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3679, https://doi.org/10.5194/egusphere-egu26-3679, 2026.

During the construction and maintenance of prefabricated box culverts in subsea tunnels, accurate assessment of the compactness of the ultra-thin bottom grouting layer is essential for ensuring overall structural stability. Ground Penetrating Radar (GPR) technology could allow non-destructive evaluation of grouting quality by capturing dielectric contrasts between media to identify hidden voids. However, real-time assessment of this 50-mm ultra-thin layer faces significant challenges, as traditional detection methods struggle to adapt to the drastic variations in dielectric properties during the rapid setting process. Furthermore, existing numerical simulations are typically based on preset defect sizes and locations, failing to reproduce the random defect features induced by grout rheology. This limitation results in a lack of high-fidelity training data for intelligent monitoring algorithms.

In this study, a physics-driven dynamic grouting scene-generation and assessment framework was proposed to address the scarcity of monitoring data for the quality of box culvert grouting. Based on the time-varying evolution laws of the grouting material from fluid to solid states, full-cycle electromagnetic characteristic parameters were obtained to establish a dynamic mapping mechanism between grouting age and radar response signals. To address the grouting diffusion mechanism in the heterogeneous structural environment of the culvert bottom, a defect scene reconstruction method was developed to consider the grouting process and the coupling between slurry rheology and gravity. This method simulates non-homogeneous and irregular void morphologies under realistic working conditions, overcoming the limitations of traditional regular geometric modeling. A high-fidelity GPR forward simulation framework was constructed to generate standardized datasets covering different setting sequences and interface contact states. Furthermore, a stepped frequency continuous wave (SFCW) simulation framework was developed to standardize data processing across different frequency bands, enabling rapid screening and localization of weak grouting zones through target-detection algorithms.

Results demonstrate that the synthetic data generated by this method effectively reflect the signal evolution patterns across different curing stages, resolving the issue of sample scarcity caused by sparse field data. Compared to static models, synthetic datasets incorporating time-varying features and rheological constraints better capture the authentic signal characteristics of early-stage defects. This indicates that improving the data generation paradigm is crucial for achieving intelligent, real-time monitoring of box culvert grouting quality.

How to cite: Zheng, W., Zhou, Y., and Wang, S.: GPR-Based Quality Assessment for Ultra-Thin Grouting Layers in Box Culverts Integrating Rheological Features and Time-Varying Electromagnetic Features , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3792, https://doi.org/10.5194/egusphere-egu26-3792, 2026.

EGU26-4095 | ECS | Orals | GI5.2

Asphalt Concrete Pavement Evaluation with GPR: A Case Study of Layer Thickness Validation and Density Prediction 

Yihan Chen, Gaurav Bhusal, Lama Abufares, and Imad Al-Qadi

Ground-penetrating radar (GPR) is at the forefront of nondestructive pavement evaluation techniques in the US, with common applications for pavements’ subsurface and surface investigations. Radar systems are effective in-depth estimation provided accurate dielectric constant is known. In this study, GPR is used for a thorough evaluation of seven different full-depth asphalt concrete (AC) segments at Illinois Certification and Research Track in Trenton, IL. The track includes three stone-matrix asphalt and four dense graded hot-mix asphalt segments with different surface characteristics namely, variation in texture and roughness. The track also includes embedded copper plates at different depths to validate GPR systems. A GPR system mounted on a vehicle was used to collect data at three different vehicular speeds (5, 10, and 20 mph). The evaluation focused on accurately estimating the dielectric constant for the different layers using their reflection amplitudes after various signal corrections. The dielectric constants are then used to predict layer thickness, AC density, and estimate depth of copper plates. The predicted results were compared to design thicknesses, core densities, and as-built copper plates layout, respectively. The results illustrate the importance of GPR signal processing and the power of GPR as a reliable evaluation tool for AC pavements.

How to cite: Chen, Y., Bhusal, G., Abufares, L., and Al-Qadi, I.: Asphalt Concrete Pavement Evaluation with GPR: A Case Study of Layer Thickness Validation and Density Prediction, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4095, https://doi.org/10.5194/egusphere-egu26-4095, 2026.

EGU26-4383 | Posters on site | GI5.2

Direction-Aware and Expert-Inspired Learning for Internal Crack Size Detection Using On-Site GPR Data 

Yiming Zhang, Zheng Tong, and Weiguang Zhang

Internal cracking in asphalt pavements develops beneath the surface and can rapidly propagate upward, threatening structural integrity and traffic safety. Crack size, especially top width, bottom width, and depth, is a key parameter for selecting maintenance strategies (e.g., grouting positioning and repaving decisions). Ground-penetrating radar (GPR) enables non-destructive subsurface inspection, yet practical crack size interpretation remains challenging due to (i) limited robustness when transferring signal–size relationships from simulations to heterogeneous field conditions, and (ii) the difficulty of directly characterizing crack size from raw GPR B-scan image features.

This study proposes an internal crack size detection network (ICSD-Net) trained on on-site GPR B-scans with interpreted crack size labels. The method targets the trapezoidal geometry of internal cracks (narrow top, wider bottom) and the fact that size-relevant information is concentrated near the hyperbolic apex of crack reflections, where confounding layer reflections often exist and conventional anchor-based/anchor-free detectors struggle with positive-sample matching.

ICSD-Net integrates three key designs. First, a deformable Cross Stage Partial (CSP) backbone improves geometric adaptability for irregular hyperbolic reflections. Second, a Directional Fusion Attention Module (DFAM) constructs direction-aware channel attention using 1D pooling along height/width and generates spatial interaction weights via directional feature broadcasting and multiplicative fusion, enhancing modeling of long-range dependencies across both sides of a hyperbola while suppressing background clutter. Third, an expert-inspired Bipartite Matching (BM) head adopts a DETR-like global set prediction strategy: the network outputs a fixed number of trapezoidal size candidates and uses Hungarian matching to select the optimal assignment between predictions and ground truth, emulating expert global reasoning on an entire B-scan.

A field dataset was built using a 3D GPR array system (24 channels, 800 MHz) from a highway rehabilitation project; signals were minimally processed (direct-wave removal and normalization). Crack size labels were derived by combining forward-model-informed relationships between reflection amplitude and crack top/bottom widths (high correlation reported) with travel-time-based depth estimation, then annotated as four-corner trapezoids on B-scans. The dataset contains 1968 labeled B-scans (small/medium/large targets) split into train/validation/test at 7:2:1.

Experiments show ICSD-Net outperforms multiple state-of-the-art baselines (including YOLO pose variants and DETR adaptations), achieving the highest mAP and mIoU with approximately 8-12% mAP improvement over the strongest baseline, while maintaining real-time feasibility. Ablation studies indicate that DFAM and the BM head contribute most to accuracy gains, improving attention focus toward the hyperbolic apex and reducing misdetections caused by layer reflections. Stability tests demonstrate consistent performance across antenna frequencies and pavement structures, supporting practical deployment. Field validation using coring measurements indicates predicted crack sizes generally meet engineering requirements, with remaining difficulty in accurately estimating bottom width for water-saturated and small cracks due to strong dielectric-contrast-induced multiple reflections and deeper-layer noise.

How to cite: Zhang, Y., Tong, Z., and Zhang, W.: Direction-Aware and Expert-Inspired Learning for Internal Crack Size Detection Using On-Site GPR Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4383, https://doi.org/10.5194/egusphere-egu26-4383, 2026.

EGU26-5246 | Posters on site | GI5.2

SCB-ADAE: An Attention-based Deep Autoencoder for Ground Penetrating Radar Signal Denoising 

jiahao liu, zheng tong, and yiming zhang

Ground Penetrating Radar (GPR) is a widely used geophysical tool for subsurface investigation, including applications in civil engineering, environmental studies, and archaeological explorations. However, GPR signals are often contaminated by various types of noise. These noise factors can significantly degrade the quality of the GPR signal. Existing denoising techniques often struggle to remove complex, non-Gaussian noise or site-specific interference effectively. To address this issue, this study proposes a novel denoising model, the Swin-Conv Block with Attention Denoising Autoencoder (SCB-ADAE), which integrates convolutional and self-attention mechanisms to enhance GPR signal denoising performance. The SCB-ADAE model consists of two key components: the Swin-Conv Block (SCB) and the Attention Denoising Autoencoder (ADAE). The SCB captures high-level features of the raw GPR signal, preserving important details while extracting local and global features. The ADAE module, enhanced with self-attention, focuses on the most relevant components of the signal, suppressing noise and preserving the core features that are essential for accurate interpretation. The process begins by passing the raw GPR signal through the SCB for feature extraction. Next, the ADAE module denoises the extracted features by utilizing self-attention mechanisms. Finally, the denoised signal is passed through a second SCB module for refinement and dimension matching with the original input signal. The model was tested on radar signals contaminated by Gaussian noise at varying levels (5 dB, 7.5 dB, and 10 dB), inhomogeneous-material noise, and real-world GPR signals, with performance evaluated using key metrics such as Signal-to-Noise Ratio (SNR), Peak Signal-to-Noise Ratio (PSNR), and Structural Similarity Index (SSIM). The SCB-ADAE model consistently outperformed existing state-of-the-art models like U-Net and Denoising Autoencoders. For example, at a noise level of 5 dB, SCB-ADAE achieved an SNR of 31.33 dB, PSNR of 38.59 dB, and SSIM of 0.9817, significantly surpassing SCUNet, which achieved lower scores. As the noise level increased, SCB-ADAE maintained superior performance, demonstrating its ability to handle higher levels of noise effectively. In tests involving radar signals with inhomogeneous-material noise, SCB-ADAE demonstrated a 146.74% improvement in SNR and a 16.65% improvement in PSNR compared to SCUNet, highlighting its capacity to address complex, site-specific noise types. In conclusion, the SCB-ADAE model is an effective solution for denoising GPR signals in noisy environments. Future work should focus on expanding training datasets to include more diverse noise types and exploring transfer learning techniques to improve model generalization across different geological environments.

How to cite: liu, J., tong, Z., and zhang, Y.: SCB-ADAE: An Attention-based Deep Autoencoder for Ground Penetrating Radar Signal Denoising, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5246, https://doi.org/10.5194/egusphere-egu26-5246, 2026.

EGU26-5371 | ECS | Orals | GI5.2

Potential of satellite spectral imagery applications for monitoring flexible pavement aging 

Giorgia Sanvitale, Luca Bianchini Ciampoli, Valerio Gagliardi, Deodato Tapete, and Andrea Benedetto

The efficiency and functionality of road networks deeply influence the economic and social development of a country. In contrast, when road infrastructure no longer fulfills the required standards, it could represent a serious concern in terms of safety of the transportations system. Indeed, during their lifetime, flexible pavements are subject to continuous aging and degradation due to both environmental factors and traffic loads. To maintain a high level of service and safety, it is essential to monitor this phenomenon to ensure timely scheduling of effective maintenance. Traditional monitoring techniques mainly consist in visual inspection of road segments along with different in situ measurements expressing the superficial condition and the bearing capacity of the pavement. Nevertheless, the final assessment of damage is often qualitative and limited to the observation points. In addition, these methods are expensive, labor intensive and time consuming and results inefficient at a large-scale level.

In this context, the use of remote sensing techniques has progressed in recent years as it offers a highly-productive nondestructive method for evaluating road conditions. These new techniques hold many advantages and provide an opportunity for frequent, comprehensive, and quantitative surveys of transportation infrastructures. Remote sensors can acquire the emitted and reflected energies of the target in different parts of the electric spectrum, and they can be used in the identification and characterization of distresses and aging processes of asphalt mixtures. These technologies can be implemented from various platforms, such as UAVs, airplanes and satellites, characterized by different resolutions and used for different applications.

In particular, the use of satellite imagery is remarkably promising as it enables continuous, large-scale observation of flexible pavement networks, with the possibility to have access to historical datasets, thereby allowing a long-term assessment of the pavement conditions. Despite the limited ground resolution characterizing most of multispectral and hyperspectral satellites, the collected imagery enables quantitative monitoring of flexible pavements through analysis of surface reflectance characteristics across visible (VIS), near infrared (NIR), and shortwave infrared (SWIR) wavelengths. In fact, in these regions variations in asphalt reflectance spectra are directly associated with material aging, oxidation, asphalt content reduction and aggregate exposure. It has been found that the reflectance spectrum tends to generally increase over time due to the aging phenomenon. In addition, the loss of hydrocarbons causes the vanishing of the absorption properties at 1700 nm and 2300 nm, while the aggregate exposure results in the appearance of absorption features at 520, 670 and 870 nm. These changes are evaluated by using two main indicators: the VIS2 (830 nm-490 nm) and the SWIR range (2120 nm-2340 nm).

This study reports on the feasibility of using satellite spectral products to monitor the aging of flexible pavements. Following a pro & cons analysis of this survey methodology compared to other techniques, the promising results obtained by an application over three large, paved areas located inside an airfield is presented. This research was conducted within the framework of I4DP_SCIENCE RESCUE_SAT project (Agreement n. 2025-2-HB.0), in collaboration with the Italian Space Agency (ASI).

How to cite: Sanvitale, G., Bianchini Ciampoli, L., Gagliardi, V., Tapete, D., and Benedetto, A.: Potential of satellite spectral imagery applications for monitoring flexible pavement aging, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5371, https://doi.org/10.5194/egusphere-egu26-5371, 2026.

EGU26-5977 | Orals | GI5.2

Experimental Evaluation of FBG Sensors for Real-Time Strain and Temperature Monitoring in Rigid Pavements 

Luca Bianchini Ciampoli, Ruggero Pinto, and Andrea Benedetto

Current pavement survey protocols adopted by airport authorities mainly rely on non-destructive testing techniques and visual inspections. Although effective in quantitatively assessing the structural condition of paved assets, these approaches present several limitations: they do not enable direct, real-time measurement of the superstructure’s reactive behavior under thermal and/or mechanical loading; they lack spatial and temporal consistency due to inspections being scheduled around operational constraints; and they offer limited capability for synergistic integration of data derived from multiple inspection sources.

To address these limitations, this study evaluates the reliability of an alternative structural health monitoring (SHM) system embedded within the primary load-bearing concrete layer of rigid pavements. Specifically, Fiber Bragg Grating (FBG) optical sensors are employed to simultaneously measure strain and temperature in a scaled concrete slab. The main objective is to assess the mechanical and thermal performance of both bare and transduced fiber optic sensors bonded to the bottom surface of the slab.

First, a static bending test conducted at constant temperature on the instrumented laboratory specimen demonstrates sensor durability and good agreement with corresponding numerical simulations. Subsequently, a uniform thermal gradient test on the free slab highlights the sensors’ high responsiveness and produces results consistent with the expected elastic thermal expansion of concrete, while also revealing material limitations related to thermal conductivity and inertia. Finally, a thermal deconvolution algorithm is applied to compensate for temperature-induced wavelength shifts, allowing the isolation of mechanically induced strains.

Overall, the proposed SHM system represents a promising and viable preliminary alternative for real-time monitoring of mechanical load conditions and thermal gradients in rigid pavements, which are increasingly challenged by rising traffic demands and extreme climate conditions.

How to cite: Bianchini Ciampoli, L., Pinto, R., and Benedetto, A.: Experimental Evaluation of FBG Sensors for Real-Time Strain and Temperature Monitoring in Rigid Pavements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5977, https://doi.org/10.5194/egusphere-egu26-5977, 2026.

EGU26-8415 | ECS | Orals | GI5.2

High-Resolution InSAR-based DEMs for Flood Hazard Analysis: Advances from the RESCUE_SAT Project 

Richard Mwangi, Valerio Gagliardi, Giorgia Sanvitale, Stefano Cipollini, Luciano Pavesi, Luca Bianchini Ciampoli, Fabrizio D'amico, Deodato Tapete, Maria Virelli, Alessandro Ursi, Andrea Benedetto, and Elena Volpi

The increasing frequency and intensity of flood events driven by ongoing climatic changes are exerting substantial pressure on ecosystems, productive activities, and the resilience of critical infrastructure. As a result, climate-change adaptation strategies are progressively focusing on mitigating their impacts. Numerical hydraulic and hydrological forecasting remains the principal tool for supporting prevention and protection policies, relying on Digital Terrain Models (DTMs), including Digital Elevation Models (DEMs), and land-cover information. In this context, satellite remote sensing has the unique ability to cover large spatial extents with high spatial resolution (below the meter scale) and, at the same time, to provide updated data with each new orbital acquisition. In hydrological modelling, coarser terrain data (approximately 10 m) are generally sufficient for simulating rainfall-runoff dynamics, whereas hydraulic models that resolve flood propagation require substantially finer spatial detail, typically on the order of 1 m.

The RESCUE_SAT project (Agreement n. 2025-2-HB.0), funded by the Italian Space Agency (ASI) under the “Innovation for Downstream Preparation for Science” (I4DP_SCIENCE) programme, integrates advanced hydrological and hydraulic analyses from the RESCUE model [1] with multi-scale satellite Earth Observation (EO) data. Its primary objective is to enhance flood-modelling capabilities by assimilating high-resolution EO information into rainfall-runoff simulations, thereby enabling a unified framework capable of representing both large-scale hydrological behaviour and local hydraulic processes, including flow interactions with structures such as bridge piers and embankments. By integrating the computational efficiency of DEM-based analyses with advanced hydrological and hydraulic modelling, RESCUE_SAT aims to generate physically based flood maps while maintaining time-effective workflows [2].

To this purpose, ASI’s COSMO-SkyMed (CSK) SAR products are processed using an InSAR approach to derive DEMs with a spatial resolution of 3 m over selected case-study areas in the Latium Region, Italy. The resulting DEM is then compared with other elevation products, including the SRTM v3 DEM (3 arc seconds, with a 90 m spatial resolution) [3] and a LiDAR-derived DEMs from the National Geoportal - MASE [4] with a spatial resolutions of 1 m. The CSK DEM is expected to enhance the detection of flood-prone areas, particularly where natural flow paths interact with infrastructure. RESCUE_SAT also incorporates ground-based GNSS and UAV surveys, integrated during calibration and validation to characterize local-scale processes in settings where infrastructure influences surface-water dynamics, thereby highlighting the value of multi-source satellite data for medium to large‑scale flood-risk assessment and infrastructure resilience.

References

[1] Pavesi, L., et al., (2022). RESCUE: A geomorphology-based, hydrologic-hydraulic model for large-scale inundation mapping. Journal of Flood Risk Management, 15(4), e12841

[2] Gagliardi, V., et al., (2025). Enhancing hydraulic risk assessment using next-generation satellite remote sensing: the RESCUE_SAT project. Vol. 13671. SPIE, 2025

[3] Farr, T. G., & Kobrick, M. (2000). Shuttle Radar Topography Mission (SRTM) produces a near-global digital elevation model. Eos, Transactions of the American Geophysical Union, 81(48), 583–585.

[4] Ministero dell’Ambiente e della Sicurezza Energetica (MASE). LiDAR data from PST-Geoportale Nazionale

 

How to cite: Mwangi, R., Gagliardi, V., Sanvitale, G., Cipollini, S., Pavesi, L., Bianchini Ciampoli, L., D'amico, F., Tapete, D., Virelli, M., Ursi, A., Benedetto, A., and Volpi, E.: High-Resolution InSAR-based DEMs for Flood Hazard Analysis: Advances from the RESCUE_SAT Project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8415, https://doi.org/10.5194/egusphere-egu26-8415, 2026.

EGU26-10415 | ECS | Orals | GI5.2

The Project “LAB_SAT”: A Laboratory for the Remote Monitoring of Environmental Safety in Built and Natural Assets 

Maryam Khazaee, Jhon Romer Diezmos Manalo, Valerio Gagliardi, Fabrizio D’Amico, Andrea Benedetto, Emanuela Panzironi, Alberto Iacovacci, Andrea Iacomoni, Bruno Monardo, Luigi D’Amato, and Laura Candela

The effective management of civil infrastructure and natural assets represents a significant challenge for local public administrations, particularly due to the need for real-time monitoring strategies to mitigate hydrogeological and structural risks. To bridge the gap between advanced remote-sensing capabilities and municipal governance, this work presents the framework of the “LAB_SAT” Project (Agreement N. 2025-9-HB.0), a pilot initiative promoted by the Italian Space Agency (ASI) under the “Innovation for Downstream Preparation for Public Administrations” (I4DP_PA) programme. The I4DP_PA programme was created with the aim of promoting the development of downstream services and applications and an active involvement of public administrations in their development and in the integration and use of satellite data within land management processes. The project is coordinated by the Municipality of Zagarolo as the lead Public Administration (PA), an Italian local authority in the Lazio Region, in partnership with the Italian Space Agency and in collaboration with two scientific partners, DICITA–Roma Tre University and the Fo.Cu.S.–Sapienza University. The main objective of the project is to establish a prototype of an operational laboratory dedicated to the assessment of environmental hazards and the monitoring of infrastructure, integrating multi-source data from satellite Earth Observation (EO), UAV platforms equipped with multispectral and LiDAR sensors, GNSS, and Terrestrial Laser Scanning (TLS). To this end, the project adopts a multi-sensor approach aimed at developing advanced downstream services, including displacement monitoring through MT-InSAR, change-detection analyses based on multispectral indices. The project integrates EO data by leveraging satellite missions, including SAR observations from the COSMO-SkyMed constellation and multispectral and hyperspectral products from the Sentinel-2 and PRISMA missions. All EO datasets will be analysed within a synergistic framework alongside ground-based information and terrestrial surveys, including GNSS monitoring, drone-based photogrammetry, and Terrestrial Laser Scanning reflectance analyses. Through the application of data-fusion algorithms and dedicated up-scaling and down-scaling techniques, the system generates environmental georeferenced composite indicators derived from multiple sources, fully interoperable with GIS environments and useful for urban planning. To assess the stability of local infrastructure, identify risks affecting strategic assets (e.g. viaducts, historical buildings) and monitor potential impacts from natural hazards such as landslides or soil degradation, specific indicators are employed, each capturing distinct dimensions of infrastructure conditions. A further key component of the project is the development of a Web-GIS digital platform that builds upon the existing framework and reaches full operational capability as one of the project’s final outputs, alongside the creation of a prototype Digital Twin. The LAB_SAT project provides an integrated platform to support planning, civil protection, and mobility decision-making in small municipalities, aiming to serve as a replicable model across Italy. By demonstrating the operational use of satellite-derived information, it enhances the capacity of PA to adopt proactive, evidence-based digital tools and to integrate remote-sensing and non-destructive testing methodologies for the sustainable management of built and natural environments.

Acknowledgements

This research is supported by the Project “LAB_SAT”, accepted and funded by the Italian Space Agency (Agreement N. 2025-9-HB.0) within the Innovation for Downstream Preparation - Public Administrations (I4DP_PA) program

How to cite: Khazaee, M., Manalo, J. R. D., Gagliardi, V., D’Amico, F., Benedetto, A., Panzironi, E., Iacovacci, A., Iacomoni, A., Monardo, B., D’Amato, L., and Candela, L.: The Project “LAB_SAT”: A Laboratory for the Remote Monitoring of Environmental Safety in Built and Natural Assets, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10415, https://doi.org/10.5194/egusphere-egu26-10415, 2026.

Historical buildings’ preservation is one the toughest challenges addressed by geoscientist in the field of Cultural Heritage as edifices’ state of conservation should be frequently monitored. This procedure becomes even more urgent in regions characterized by seismic events, since medium-to-high magnitude earthquakes might determine significant and expensive damages. The most common effects of degradation can be investigated with geophysical methodologies since both chemical weathering and mechanical deterioration generally ensure sufficient contrasts of the surveyed physical parameters (e.g. electrical resistivity and relative permittivity). In particular, Electrical Resistivity Tomography (ERT) and Ground Penetrating Radar (GPR) methods are commonly selected for their logistical simplicity, still granting high resolution results relatively quickly [1] with a non-destructive approach. The case study here presented involves Castellina Museum, an important medieval building in the city of Norcia (Umbria region, Central Italy). Being situated in an active seismic area, this edifice has faced several reconstructions due to the medium-to-high magnitude earthquakes occurred in the last centuries like in the case of 2016-2017 Central Italy seismic sequence when a 6.5 Mw mainshock [2] caused fatalities and damages to the buildings around Norcia. Therefore, to evaluate both the state of conservation and potential aftershocks damages, multi-methodological non-destructive geophysical surveys were conducted over a significant internal masonry wall which location, according to historical documentations, suggests its correspondence to the façade of a previous building, named “Palazzo del Podestà”. An intensive GPR campaign was carried out to evaluate the geometrical arrangement of constructive elements forming the medium. First results provided a peculiar GPR signature, confirming the expected heterogeneous texture and size of such blocks, similarly to the exposed sectors of the wall. However, from the basal floor, electromagnetic signal attenuation occurred over a large portion of the wall. Therefore, ERT was then employed to investigate the variation of electrical parameters [3]. This survey confirmed that the area affected by strong electromagnetic attenuation, are also characterized by electrical resistivity values significantly lower than the ones of neighbouring zones. Therefore, further investigations are needed to better understand the reasons behind this process. This study underlines the importance of employing complementary geophysical methods to achieve a deeper understanding of the studied problem improving the quality of the interpretation needed to define strategic planes for preservation of Cultural Heritages buildings.

 

Reference

[1] Ercoli, M.; Brigante, R.; Radicioni, F.; Pauselli, C.; Mazzocca, M.; Centi, G.; Stoppini, A. Inside the Polygonal Walls of Amelia (Central Italy): A Multidisciplinary Data Integration, Encompassing Geodetic Monitoring and Geophysical Prospections. Journal of Applied Geophysics 2016, 127, 31–44, doi:10.1016/j.jappgeo.2016.02.003.

[2] Porreca, M.; Minelli, G.; Ercoli, M.; Brobia, A.; Mancinelli, P.; Cruciani, F.; Giorgetti, C.; Carboni, F.; Mirabella, F.; Cavinato, G.; et al. Seismic Reflection Profiles and Subsurface Geology of the Area Interested by the 2016–2017 Earthquake Sequence (Central Italy). Tectonics 2018, 37, 1116–1137, doi:10.1002/2017TC004915.

[3] Leucci, G. Ground Penetrating Radar: The Electromagnetic Signal Attenuation and Maximum Penetration Depth. Scholarly Research Exchange 2008, 2008, 1–7, doi:10.3814/2008/926091.

How to cite: Alaia, G., Ercoli, M., Mazzocca, M., and Cavalagli, N.: Multi-methodological geophysical characterization for the preservation of Cultural Heritage in seismic area: the case of Museo della Castellina in Norcia (Central Italy), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11757, https://doi.org/10.5194/egusphere-egu26-11757, 2026.

EGU26-12107 | ECS | Posters on site | GI5.2

A Multi-Source Non-Destructive Testing Survey for Digital Modelling and Reconstruction: The Case Study of Palazzo Ripetta in Rome 

Jhon Romer Diezmos Manalo, Valerio Gagliardi, Andrea Vennarucci, Luca Bianchini Ciampoli, Pietro Meriggi, Sara Fares, Gianmarco de Felice, and Andrea Benedetto

Conventional visual inspection of civil infrastructure and cultural heritage is limited by subjectivity, restricted accessibility, and safety risks. Developing an integrated methodology to accurately reconstruct and survey existing structures and infrastructures, with millimetric geometric accuracy and reliable information on material conservation conditions, is therefore essential to overcoming these constraints. With the progressive deterioration of historic structures and major cultural-heritage assets, including bridges, monuments, historic buildings, and aging roadways, the need for highly accurate measurement and documentation has become increasingly critical. To this end, the use of multi-source Non-Destructive Testing (NDT) techniques for the acquisition of fast and accurate geometric and radiometric information is a necessity. This research proposes an integrated geomatic workflow designed to digitize complex built environments through multi-sensor data integration, enabling advanced analysis within immersive virtual environments. The methodological approach relies on a robust topographic reference frame established via Global Navigation Satellite Systems (GNSS) and high-precision Total Stations, ensuring the global georeferencing required for engineering reliability. To capture the full complexity of the assets, the study employs a synergistic acquisition strategy. Terrestrial Laser Scanning (TLS) is a process of generating a high-resolution point cloud representing the geometry of the ground and other features that can be reached from ground level, while simultaneously employing Unmanned Aerial Vehicles (UAVs) to address any occluded areas caused by the ground perspective and enabling the inspection of buildings' upper levels and structural components. The UAV equipment consists of an optical-camera payload that enables millimetric-resolution acquisition for high-definition photogrammetric modelling. 
All these multi-source surveying tools were employed to reconstruct a digital model of a real architectural complex, the Bernini Hall, now incorporated into the Palazzo Ripetta ensemble in Rome, Italy. Within this context, one of the most significant historic and artistic spaces within the building preserves a refined architectural and cultural heritage of substantial value. The multi-source datasets were subsequently post-processed for georeferencing and for the registration of the different acquisitions, resolving geometric discrepancies and producing a single, multi-layered 3D point cloud. This digital model forms the basis for structural analysis, also enabling the assessment deformation reconstruction, with millimetric accuracy. The novelty of this framework lies in its shift from traditional static digital-model analysis to immersive visualization. The digital model, derived from the integration of UAV imagery through photogrammetric reconstruction and LiDAR point-cloud data by TLS, is imported into a Virtual Reality (VR) environment using Unity®, a dedicated software optimized for high-fidelity rendering, enabling immersive exploration and navigation within the model, with millimetric accuracy consistent with the NDT-based survey. The use of Head-Mounted Displays (HMDs) enables users to experience a fully immersive digital representation, navigating the space as if physically present. The reconstructed digital model improves the accuracy of inspections in critical or hard-to-access areas, opens new ways for structural-health-monitoring efficiency and broadens opportunities for the valorization and remote accessibility of the built environment.

How to cite: Manalo, J. R. D., Gagliardi, V., Vennarucci, A., Bianchini Ciampoli, L., Meriggi, P., Fares, S., de Felice, G., and Benedetto, A.: A Multi-Source Non-Destructive Testing Survey for Digital Modelling and Reconstruction: The Case Study of Palazzo Ripetta in Rome, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12107, https://doi.org/10.5194/egusphere-egu26-12107, 2026.

EGU26-12184 | Orals | GI5.2

Numerical and Experimental Analysis of Multistatic GPR Systems for Subsurface Inspection 

Carlo Noviello, Mehdi Masoodi, Gianluca Gennarelli, Giovanni Ludeno, Giuseppe Esposito, Ilaria Catapano, and Francesco Soldovieri

Ground-Penetrating Radar (GPR) is a non-invasive sensing technology [1] that exploits the propagation of electromagnetic pulses to investigate opaque media, such as soil, sand, ice, concrete, asphalt, and many others. GPR enables the detection and characterization of dielectric anomalies arising from interfaces, voids, cracks, moisture ingress, reinforcement corrosion, and variations in layer thickness. Owing to its non-destructive nature, GPR has become a key tool for the structural health monitoring of critical infrastructures (e.g. bridges, tunnels, roads, railways, and buildings) thereby contributing to the sustainability, safety, and resilience of the built environment.

Although GPR is a well-established technology employed in a wide range of operational contexts, its performance can be significantly degraded by the presence of noise and clutter, especially when operating in contactless mode and in complex scenarios, f.i. when mounted on mobile vehicles, unmanned aerial platforms, or robotic systems [2]. To overcome these limitations, advanced measurement configurations employing multiple transmitting and receiving antennas have recently been proposed [3]. At the state of art, multistatic radar technology represents a promising solution for mitigating signal disturbances and enhancing subsurface imaging capabilities [4]. However, this technology entails a substantial increase in data volume and computational complexity, thus requiring the development of efficient and robust signal processing and image reconstruction strategies. Within this framework, a key challenge lies in the identification of suitable measurement setups that achieve an optimal trade-off between imaging performance and computational cost.

In this contribution, a performance assessment of different multistatic antenna configurations operating in a three-dimensional free-space scenario and consisting of a single transmitting antenna and multiple receiving antennas is considered. First, a numerical analysis will be conducted to assess the imaging capabilities of the system. Then, experimental results obtained under controlled laboratory conditions will be presented to validate the proposed imaging approach and identify the configurations that provide the best compromise between reconstruction quality and computational cost.

References

  • Daniels, David J., ed. Ground Penetrating Radar. Vol. 1. Iet, 2004.
  • Catapano I., Gennarelli G., Ludeno G., Noviello C., Esposito G., Soldovieri F., "Contactless Ground Penetrating Radar Imaging: State of the art, challenges, and microwave tomography-based data processing," in IEEE Geoscience and Remote Sensing Magazine, vol. 10, no. 1, pp. 251-273, March 2022, doi: 10.1109/MGRS.2021.3082170.
  • Masoodi, M.; Gennarelli, G.; Noviello, C.; Catapano, I.; Soldovieri, F. Performance Assessment of Multistatic/Multi-Frequency 3D GPR Imaging by Linear Microwave Tomography. Sensors 2025, 25, 6467.
  • Noviello, C.; Braca, P.; Maresca, S. Chapter 5—Radar Networks. In Photonics for Radar Networks and Electronic Warfare Systems; SciTech Publishing, Inc.: Raleigh, NC, USA, 2019; p. 111.

How to cite: Noviello, C., Masoodi, M., Gennarelli, G., Ludeno, G., Esposito, G., Catapano, I., and Soldovieri, F.: Numerical and Experimental Analysis of Multistatic GPR Systems for Subsurface Inspection, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12184, https://doi.org/10.5194/egusphere-egu26-12184, 2026.

EGU26-13903 | ECS | Orals | GI5.2

Risk assessment of bridges affected by subsidence and landslides using ground and spaceborne monitoring: a global study 

Dominika Malinowska, Pietro Milillo, Cormac Reale, Chris Blenkinsopp, and Giorgia Giardina

Bridges are a core element of transport systems, enabling connectivity and supporting access to employment, education, medical care and emergency response. Despite this central role, they are also among the most fragile assets in these networks, as they are frequently exposed to natural hazards whose occurrence and intensity are expected to grow under changing climatic conditions. Although assessing geo-hazard risk to bridges is essential for meeting the United Nations Sustainable Development Goals, current risk evaluation practices rarely account for how structural vulnerability evolves over time. In particular, they overlook the contribution of continuous monitoring technologies such as Structural Health Monitoring (SHM) sensors and Interferometric Synthetic Aperture radar (InSAR), which can provide ongoing information on bridge condition. Furthermore, while SHM installations remain limited, the global capacity of InSAR to complement these systems for bridge surveillance has not yet been systematically quantified.

This study introduces a new framework for assessing bridge geo-hazard risk worldwide that explicitly incorporates the availability of both ground-based SHM and satellite-derived monitoring. The assessment integrates subsidence and landslide hazards with measures of exposure and structural vulnerability.

A global analysis of satellite monitoring coverage reveals a substantial shortfall in current observation capability. Only a small fraction of long-span bridges is equipped with SHM systems, whereas InSAR observations from Sentinel-1 could potentially cover a far larger share of the global bridge inventory. Expanding the use of this spaceborne data could therefore lower overall geo-hazard risk and reduce the number of bridges categorised as high risk. Many of the structures that would remain in the high-risk category are also well-suited to satellite-based monitoring, underlining the value of InSAR for improving safety and resilience, particularly in low-income and resource-constrained regions. By linking risk with monitoring suitability, the proposed framework highlights that the presence of SHM and InSAR sensors enables more dynamic and time-sensitive risk evaluation, providing practical guidance for prioritising satellite monitoring, SHM deployment, and on-site inspections within a risk-informed decision-making process.

How to cite: Malinowska, D., Milillo, P., Reale, C., Blenkinsopp, C., and Giardina, G.: Risk assessment of bridges affected by subsidence and landslides using ground and spaceborne monitoring: a global study, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13903, https://doi.org/10.5194/egusphere-egu26-13903, 2026.

EGU26-15105 | ECS | Orals | GI5.2

Evaluating an Extended Reality Prototype for Multi-Modal Geophysical Data Visualisation Through Expert Stakeholder Interviews 

Elikem Doe Atsakpo, Francesco Mercogliano, Stephen Uzor, Saeed Parnow, Atiyeh Ardakanian, Andrea Barone, Filippo Accomando, Raffaele Castaldo, Ilaria Catapano, Pietro Tizzani, and Fabio Tosti

The interconnectedness and complexity of subsurface structures present challenges for their identification and visualisation. To address this, geophysicists routinely integrate multiple non-destructive sensing techniques to map underground utilities. These resulting sensor outputs are predominantly two-dimensional (2D) products, typically visualised as maps and sections, using 2D Geographic Information System (GIS) software [1], or more recently, as three-dimensional (3D) objects that encode depth information. However, despite the use of 3D representations, these visualisations are still commonly viewed via 2D projection media, such as monitors or mobile screens. Since these visualisations directly inform professional interpretation, it is essential to understand how stakeholders, those responsible for analysing, validating, and acting on geophysical data, engage with these platforms in practice.

Advances in three-dimensional visualisation technologies, such as Extended Reality (XR), offer new opportunities to overcome these limitations. XR environments enable the integration of heterogeneous geophysical datasets within a single, interactive spatial framework, potentially enhancing spatial comprehension and interpretative accuracy. Recent studies have consequently begun exploring XR applications for subsurface and geophysical data visualisation [2]. A recent study [3] visualised drone-based Ground Penetrating Radar (GPR) and magnetometric data in a Virtual Reality (VR) prototype, identifying frame-rate instability and high GPU utilisation as key technical limitations.

However, technical performance alone does not determine the success of a visualisation tool; stakeholder perspectives are critical to ensuring XR outputs align with the analytical requirements and decision-making practices of geophysical professionals. Building on prior work, the present study extends this prototype for preliminary user testing with six expert geophysical stakeholders. These participants were selected based on their extensive professional experience, ensuring the evaluation reflects real-world interpretative conditions rather than abstract usability testing. Feedback collected through semi-structured interviews was analysed thematically, yielding four key insights: (1) the necessity of adjustable colour maps to enhance data intensity interpretation; (2) the requirement for interactive selection of colour values to reveal metadata; (3) the importance of stakeholder-centred visualisation design; and (4) the implementation of a data catalogue to allow selective dataset visualisation.

Future work will focus on refining the prototype based on these expert recommendations. This iterative process will involve a second round of evaluation to validate the updates, followed by pilot testing with broader stakeholder groups to evaluate the tool's effectiveness in real-world settings.

 

Keywords: Extended Reality; Multi-sensor Datasets; Human-in-the-loop; Data Visualisation

 

Acknowledgements: This research was funded by the Vice-Chancellor’s PhD Scholarship at the University of West London.

 

References

[1] QGIS.org, "QGIS Geographic Information System," Http://Www.Qgis.Org, vol. 2026, 2026.

[2] M. Janeras, J. Roca, J.A. Gili, O. Pedraza, G. Magnusson, M.A. Núñez-Andrés and K. Franklin, "Using Mixed Reality for the Visualization and Dissemination of Complex 3D Models in Geosciences—Application to the Montserrat Massif (Spain)," Geosciences, vol. 12, -10-07. 2022.

[3] E.D. Atsakpo, F. Mercogliano, S. Uzor, P. Saadati, A. Barone, F. Accomando, R. Castaldo, I. Catapano, P. Tizzani and F. Tosti, "Visualising Multi-Modal Geophysical Data in Extended Reality," 2025 6th International Conference on Computer Vision and Data Mining (ICCVDM), pp. 195, -09-12. 2025.

How to cite: Doe Atsakpo, E., Mercogliano, F., Uzor, S., Parnow, S., Ardakanian, A., Barone, A., Accomando, F., Castaldo, R., Catapano, I., Tizzani, P., and Tosti, F.: Evaluating an Extended Reality Prototype for Multi-Modal Geophysical Data Visualisation Through Expert Stakeholder Interviews, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15105, https://doi.org/10.5194/egusphere-egu26-15105, 2026.

EGU26-15445 | ECS | Posters on site | GI5.2

Investigating Subsurface Failure Mechanisms and Mud Pumping in Rigid Airfield Pavements Using Ground Penetrating Radar: A Collaborative Study at Heathrow Airport 

Saeed Parnow, Morven Bolton, Richard Fairley, Alkmini Karastamati, Richard Smith, Jose Fernandez, and Fabio Tosti

The condition of airfield pavements plays a central role in ensuring the safety and efficiency of airport operations. Compared with highway pavements, those on runways and taxiways are exposed to far heavier and more repetitive dynamic loading from aircraft. Over time, these loads can trigger complex deterioration processes that are not easily identified through surface inspection. Among these, mud pumping is particularly damaging, as it accelerates the structural deterioration of rigid concrete slabs and reduces their service life.

Mud pumping develops when water accumulates at the interface between a concrete slab and its sub-base or subgrade. Under repeated high-magnitude loads, a slurry of water and fine soil particles is expelled through joints and cracks. This movement of material results in subsurface voids, uneven support, increased slab deflection, and, eventually, cracking or differential settlement (sinking) of concrete bays. Previous studies have highlighted that knowing the location and extent of these voids is critical for effective slab stabilisation [1]. At Heathrow Airport, this mechanism has led to several cases of significant cracking and premature pavement distress, prompting a detailed investigation into its causes and distribution.

This study presents a collaborative research framework between academia and Heathrow Airport’s asset management team to assess the capability of Ground Penetrating Radar (GPR) as a primary non-destructive method for detecting early-stage pavement decay. Although Heathrow has identified specific areas of concern, such as the Charlie taxiway, the failure mechanisms often remain hidden until surface damage becomes advanced. By utilising GPR, this study aims to characterise the dielectric contrasts associated with moisture accumulation and subsurface voids that typically precede active mud pumping. The effectiveness of GPR for mapping these internal condition variations has been well-documented, particularly in the characterisation of pavement layer interfaces and moisture content [2].

The methodology focuses on high-resolution subsurface imaging to map the internal condition of concrete bays showing unexpected deterioration patterns. The flexibility of GPR enables the use of different frequencies to balance penetration depth with the resolution required to identify features such as thin delamination layers and incipient voids [3].

The long-term goal is to support a shift from reactive maintenance to a proactive, data-driven management strategy. By identifying the geophysical indicators of mud pumping and structural voids, the study aims to provide a diagnostic approach that can help forecast future failure areas, enhance maintenance planning, and extend the operational lifespan of critical airfield infrastructure.

 

Keywords: Ground Penetrating Radar (GPR); Airfield Pavement Management; Mud Pumping; Non-Destructive Testing (NDT)

 

References

[1] Maser, K. R. (2013). Use of GPR for Subsurface Pavement Investigations of 23 Airports in South Carolina, Proceedings Ninth International Conference on BCRRA, Vol 1.

[2] Al-Qadi, I. L., & Lahouar, S. (2005). Measuring Layer Thicknesses with GPR – Theory to Practice, Vol. 19, 10, 763-772.

[3] Benedetto, A., Tosti, F., Bianchini, L., & D’Amico, F. (2018). An Overview of Ground-penetrating Radar Signal Processing Techniques for Road Inspections, Vol. 32, 201-209.

How to cite: Parnow, S., Bolton, M., Fairley, R., Karastamati, A., Smith, R., Fernandez, J., and Tosti, F.: Investigating Subsurface Failure Mechanisms and Mud Pumping in Rigid Airfield Pavements Using Ground Penetrating Radar: A Collaborative Study at Heathrow Airport, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15445, https://doi.org/10.5194/egusphere-egu26-15445, 2026.

EGU26-16398 | Posters on site | GI5.2

Thermal Analysis for Resilient Transport Infrastructure: A Downscaling Approach Using Satellite EO Data and UAV 

Andrea Benedetto, Valerio Gagliardi, Jhon Romer Diezmos Manalo, and Nicol Cannone

In the context of the ongoing climate crisis, the Urban Heat Island (UHI) phenomenon represents one of the most critical challenges for the sustainability of the built environment. Critical transport infrastructures, such as highways, railways, and airports, play a pivotal role in this process. Due to their extension and to the thermophysical properties of the construction materials employed (e.g., asphalt, concrete), they act as significant thermal collectors. On the other hand, in urban areas transport infrastructures negatively affect the local microclimate, thereby reducing the resilience of urban areas.

 

In this context, satellite Earth Observation (EO) has emerged as a promising tool for monitoring temperature variations [1]. However, temperature measurement in the context of transport infrastructure remains challenging due to the limitations imposed by the spatial resolution of satellite sensors. The primary issue concerns the limited spatial resolution of currently available thermal satellite sensors (with a native resolution of 100 m, resampled to 30 m), such as the TIRS instrument on Landsat 8/9 [2]. While these sensors provide accurate radiometric data, they lack the geometric detail required to analyze specific transportation assets. To overcome this limitation, this research proposes an innovative methodology based on a multi‑scale thermal downscaling procedure, implemented within the Google Earth Engine platform and applied on a real‑scale parking area scenario.

 

The adopted methodology relies on the synergistic integration of multi‑scale satellite data, following the approach implemented by [3]. This study exploits the well‑established relationship between Land Surface Temperature (LST) and land‑cover metrics, including the Normalized Difference Vegetation Index (NDVI), the Normalized Difference Built‑up Index (NDBI), and the Normalized Difference Water Index (NDWI). A multiple linear regression model was first defined using spectral indices and LST derived from Landsat 8 data; this model was then applied using the corresponding spectral indices extracted from Sentinel‑2 imagery [4] to predict LST at a spatial resolution of 10 m. Subsequently, a second downscaling step was performed by applying a multi‑regression approach based on RGB bands from Sentinel‑2 and UAV imagery, enabling the estimation of surface temperature at sub‑meter resolution. Through this two‑stage procedure, the resolution of LST maps was significantly enhanced, achieving a resolution commensurate with the scale of transport infrastructure. This approach was applied to a parking area in Rome, demonstrating the potential of a sequential thermal downscaling procedure that progressively refines satellite‑derived temperatures using higher‑resolution Sentinel‑2 data and UAV imagery. The results confirm that thermal analysis based on satellite EO data and downscaling techniques is a promising, effective, and cost‑efficient method for assessing infrastructure resilience.

 

References

[1] Almeida CR, et al,. Study of the Urban Heat Island (UHI) Using Remote Sensing Data/Techniques: A Systematic Review. Environments 2021;8(10)

[2] Landsat Official Website. Accessed 01-2025. https://landsat.gsfc.nasa.gov/satellites/landsat-9/landsat-9-instruments/landsat-9-spectral-specifications/

[3] Onačillová, K. et al.. Combining Landsat 8 and Sentinel-2 Data in Google Earth Engine to Derive Higher Resolution Land Surface Temperature Maps in Urban Environment. Remote Sens. 2022, 14, 4076.

[4] European Space Agency - Sentinel-2 User Handbook, (2015)

How to cite: Benedetto, A., Gagliardi, V., Manalo, J. R. D., and Cannone, N.: Thermal Analysis for Resilient Transport Infrastructure: A Downscaling Approach Using Satellite EO Data and UAV, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16398, https://doi.org/10.5194/egusphere-egu26-16398, 2026.

Seasonal variations in environmental conditions strongly influence evapotranspiration (ET) and its components, evaporation (E) and transpiration (T), thereby directly affecting agricultural water use. Understanding how these environmental factors regulate ET dynamics is essential for improving water management in semi-arid agricultural regions of India. The study is carried out in Sangareddy district of Telangana, India during the Kharif and Rabi seasons (2024). ET was estimated for both Kharif and Rabi seasons using satellite-based energy balance modelling and divided into its E and T components. To comprehend their impact on surface–atmosphere interactions and crop water consumption dynamics, the seasonal environmental impact on ET is analysed in connection to shifting climatic conditions. Temporal variations of major variables including air temperature (Ta), vapour pressure deficit (VPD), solar radiation (Rs), and precipitation (P) are investigated in this study. Cumulative precipitation distribution during establishment, flowering, growth, and maturity stages of the crop is estimated and compared with average crop water requirement. Furthermore, highlighting the need for irrigation, particularly during the establishment and flowering stages, avoiding crop water stress was observed. During the crop cycle in both seasons, mean leaf area index (LAI) and soil moisture content were also evaluated for the studied region. The analysis shows a significant seasonal contrasts in ET magnitude and its partitioning, with transpiration dominating during peak crop growth under favourable moisture conditions, while evaporation contributed more during early growth stages and dry spells. The results demonstrate that, higher air temperature, vapour pressure deficit, and solar radiation during the Rabi season enhanced atmospheric demand, leading to increased irrigation requirements, particularly during establishment and flowering stages. Thus, these findings emphasises the utility of satellite-based ET partitioning for identifying water-stress-prone growth stages and optimizing irrigation strategies in semi-arid agricultural regions.

Keywords: Evapotranspiration; ET partitioning; environmental variability; satellite imagery'; semi-arid agriculture

How to cite: Moharana, S. and Nithin, E.: Environmental Controls on Evapotranspiration Partitioning in a Semi-Arid Agricultural Region of Telangana, India, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16546, https://doi.org/10.5194/egusphere-egu26-16546, 2026.

EGU26-16577 | ECS | Posters on site | GI5.2

Earth Observations into Urban Resilience: Exploring the Nexus between Nature-based Solutions, Infrastructure and Climate Interactions 

Suman Kumari, Tesfaye Tessema, Atiyeh Ardakanian, David Daou, and Fabio Tosti

Ramsar sites are Wetlands of International Importance under the 1971 Convention. They function as premier nature-based solutions (NbS) by safeguarding ecosystems and delivering multifaceted services essential for sustainable development. The key services include flood regulation, water treatment, carbon sequestration, shoreline prevention, biodiversity support, providing space for recreational activities, generating local employment opportunities, and directly aligning with the UN Sustainable Development Goals (SDGs) [1].

The study aims to assess and analyse the trends of wetland dynamics, which are combinedly influenced by increased urban pressure, airport expansion, associated infrastructure, and climate variability. These overlapping stressors create a complex socio-ecological system that requires integrated monitoring approaches. To address this, the research applies Earth Observation (EO) data for the South West London Waterbodies Ramsar site [2]. This is a part of the Thames River basin and supports a significant waterfowl population and functions as a wetland ecosystem adjacent to a major aviation infrastructure.

The study explores Sentinel collections, Landsat series, land use land cover (LULC) and ancillary data to identify patterns and effectively capture and monitor wetland dynamics [3] [4], water quality [4], and changes in extent and overall condition [5].

The study emphasises the importance of EO for monitoring wetlands within complex urban infrastructure landscapes. This study will demonstrate how EO-derived insights can support stakeholders, policymakers, and decision-makers in designing and developing evidence-based climate adaptation and mitigation strategies, enabling targeted NbS interventions to strengthen system-wide resilience.

 

Keywords: NbS, Ramsar site, Wetlands, Climate Resilience, Urban Infrastructure, Earth Observation

 

Acknowledgments: This research was funded by the Vice-Chancellor’s PhD Scholarship at the University of West London. Sincere thanks to the following for their support: The Lord Faringdon Charitable Trust, The Schroder Foundation, The Cazenove Charitable Trust, The Ernest Cook Trust, Sir Henry Keswick, Ian Bond, P. F. Charitable Trust, Prospect Investment Management Limited, The Adrian Swire Charitable Trust, John Swire Charitable Trust, The Samuel Storey Family Charitable Trust, The Tanlaw Foundation, and The Wyfold Charitable Trust.

 

References

[1] Ramsar, "Scaling up wetland conservation, wise use and restoration to achieve
the Sustainable Development Goals," pp. 1–13, 2018. Available: https://www.ramsar.org/sites/default/files/documents/library/wetlands_sdgs_e.pdf.

[2] Ramsar. Ramsar Sites Information Service. Available: https://rsis.ramsar.org/ris/1038?__goaway_challenge=meta-refresh&__goaway_id=67266e1927adeb4042d00a7e1a15f9c3..

[3] Z. Wang et al, "Monitoring the Wetland of the Yellow River Delta by Combining GF-3 Polarimetric Synthetic Aperture Radar and Sentinel-2A Multispectral Data," Front. Ecol. Evol., vol. 10, 2022. Available: https://www.frontiersin.org/journals/ecology-and-evolution/articles/10.3389/fevo.2022.806978/full. DOI: 10.3389/fevo.2022.806978.

[4] M. Singh and R. Sinha, "Hydrogeomorphic indicators of wetland health inferred from multi-temporal remote sensing data for a new Ramsar site (Kaabar Tal), India," Ecological Indicators, vol. 127, 2021. Available: https://www.sciencedirect.com/science/article/pii/S1470160X21004040. DOI: 10.1016/j.ecolind.2021.107739.

[5] W. Chaoyong et al, "SAR image integration for multi-temporal analysis of Lake Manchar Wetland dynamics using machine learning," Sci Rep, vol. 14, (1), pp. 14, 2024. Available: https://www.nature.com/articles/s41598-024-76730-1. DOI: 10.1038/s41598-024-76730-1.

How to cite: Kumari, S., Tessema, T., Ardakanian, A., Daou, D., and Tosti, F.: Earth Observations into Urban Resilience: Exploring the Nexus between Nature-based Solutions, Infrastructure and Climate Interactions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16577, https://doi.org/10.5194/egusphere-egu26-16577, 2026.

EGU26-18556 | Posters on site | GI5.2

Promoting Community Engagement for Trees Through Technology-Informed Practices: From Framework to Guidance 

Fabio Tosti, Becky Porter, Dale Mortimer, Atiyeh Ardakanian, Delphina Darko, Elikem Doe Atsakpo, Suman Kumari, Sangeetha Nesiah, Malte Ressin, Parisa Saadati, and Tesfaye Tessema

Community engagement is a fundamental pillar of sustainable urban forestry, essential for expanding canopy cover and promoting a societal "stewardship for trees". While traditional outreach aligns urban development with local priorities, it often faces challenges in continuity and representation, frequently resulting in "engagement fatigue" [1]. There is currently a major missed opportunity to use digital tools to connect expert tree-care decisions with public input. Although smart-city technologies offer new ways to communicate, complex tech can accidentally reinforce disparities in egagement if it is not managed carefully [2].

To address this, the London Tree Officers Association (LTOA) established a Working Party on “Promoting Community Engagement for Trees Through Technology-Informed Practices.” This initiative aims to develop strategic pathways toward new guidelines that empower local stakeholders in tree management, improving socio-economic resilience and environmental stewardship. Central to this mission is the "Technological Level of Preparedness" (TLOP) model, which categorises community groups by technology familiarity to ensure equitable and accessible engagement.

The initiative is driven by ongoing, data-informed collaboration among a diverse range of urban forestry stakeholders. Regular meetings enable the Working Party to integrate expert knowledge with local insights to better understand the environmental and social priorities, such as urban cooling and biodiversity, that guide tree management. Recent deliberations also emphasis that content quality is key to maintaining interest, shifting focus from simple planting to long-term stewardship.

To support the formulation of these guidelines, the Working Party is currently shaping potential case studies to test technologies tailored to different identified TLOP levels. Proposed initiatives include the use of gamification via mobile applications to engage younger demographics; for example, trivia games and interactive digital badges could be implemented to incentivise physical interaction with urban nature [4]. Additionally, the application of immersive technologies, such as Augmented Reality (AR) and Virtual Reality (VR), is being explored to help visualise urban regeneration, making abstract environmental data tangible [5]. The initiative also explores enhancing visualisations of canopy health through geospatial and remote sensing technologies.

By exploring how to integrate traditional methods, like guided tree walks, with these new digital tools, the initiative seeks to build a strong foundation. This framework aims to provide the groundwork that could eventually lead to formal guidance for practitioners.

Keywords: Community Engagement; Urban Forestry; Digital Inclusion; Immersive Technology; Geospatial Data.

 

Acknowledgements: This work is supported by the London Tree Officers Association (LTOA) Working Party on Community Engagement.

 

References

[1] Nitoslawski, S. & Konijnendijk, C. (2022). The Emergence of Smart Urban Forestry: Challenges and Opportunities in the Digital Age. Arboric. & Urban For., 48(2).

[2] Russo, A. Towards Nature-Positive Smart Cities: Bridging the Gap Between Technology and Ecology. (2025). Smart Cities, 8(1):26.

[3] Srinurak, N. et al. (2024). Smart Urban Forest Initiative: Nature-Based Solution and People-Centered Approach for Tree Management in Chiang Mai, Thailand. Sustainability, 16(24), 11078.

[4] Nand, K., Baghaei, N., Casey, J. et al. (2019). Engaging children with educational content via Gamification. Smart Learn. Environ. 6, 6.

[5] Zürcher, R. et al. (2023). Advancing Forest Monitoring and Assessment Through Immersive Virtual Reality. AGILE: GIScience, 4,1-12.

How to cite: Tosti, F., Porter, B., Mortimer, D., Ardakanian, A., Darko, D., Doe Atsakpo, E., Kumari, S., Nesiah, S., Ressin, M., Saadati, P., and Tessema, T.: Promoting Community Engagement for Trees Through Technology-Informed Practices: From Framework to Guidance, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18556, https://doi.org/10.5194/egusphere-egu26-18556, 2026.

EGU26-19237 | ECS | Orals | GI5.2

Multi-modal Remote Sensing and in-situ Sensors Integration for Advanced Airport Asset Monitoring 

Tesfaye Tessema, Atiyeh Ardakanian, Morven Bolton, Richard Fairley, Alkmini Karastamati, Richard Smith, Jose Fernandez, and Fabio Tosti

Runways and taxiways constitute a vital component of an airport hub. They are engineered to endure for decades; however, there are reports indicating that they may deteriorate prior to the completion of their designated lifespan, as seen in cases where 30-year designs fail within the first decade. Such deterioration includes premature distress indicators such as rutting, mud pumping, concrete slab sinking, and reflective cracking, often linked to specific material factors such as 100% Ordinary Portland Cement (OPC) design mixes. These issues can be influenced by factors such as subgrade condition, drainage quality, seasonal moisture variations, and geotechnical stability. Furthermore, factors such as ambient temperature and construction workmanship can significantly reduce the design life; if the pavement is not cured properly or poured correctly, it becomes highly susceptible to early-stage failure.

Present monitoring practices are predominantly reliant on limited in-situ testing and visual surveys, which often fail to capture the rate of deterioration at a network-wide scale or the root cause of early pavement failure. The advancement of remote sensing technologies, including Synthetic Aperture Radar (SAR) time-series, provides a reliable instrument for the precise monitoring of millimetric-scale deformations across extensive airport areas [1]. However, a comprehensive linkage between SAR observations, pavement failure mechanics, surface distress evolution, and long-term asset management decision making is still at an early stage.

In this study, we propose a prototype multi-sensor framework designed for the early detection and characterisation of airport pavement failures. This framework integrates satellite InSAR technology for long-term and seasonal deformation time-series analysis, high-resolution optical imagery for surface distress mapping, and incorporates detailed in-situ pavement investigations. The methodology examines the correlation between seasonality of SAR displacement and ambient temperature, weather, or traffic records to separate consolidation, settlements, and thermoelastic responses. The framework evaluates the utility of these data streams to identify trend profiles that may help characterise the speed of deterioration in "difficult" sections, such as those experiencing mud pumping or sinking bays [2]. The distress metrics and their temporal evolution are extracted from co-registered optical products to track the progression of visible surface damage. In-situ observations serve to validate and provide structural and materials ground truth [3]. The combination of multi-source data facilitates deformation features relating to environmental drivers. These data sources are essential to better understand the pavement states and different scenarios of changes over time. This approach supports asset owners in moving toward data-driven pavement management and optimal budget allocation.

 

 

Keywords: InSAR Time-Series Analysis; Airport Asset Management; Pavement Deterioration Modelling; Multi-modal Remote Sensing; Infrastructure Resilience

 

References

[1] Ferretti, A., Prati, C., & Rocca, F. (2001). Permanent scatterers in SAR interferometry. IEEE Transactions on Geoscience and Remote Sensing, 39(1), 8–20.

[2] Gagliardi, V.; Bianchini Ciampoli, L.; Trevisani, S.; D’Amico, F.; Alani, A.M.; Benedetto, A.; Tosti, F. Testing Sentinel-1 SAR Interferometry Data for Airport Runway Monitoring: A Geostatistical Analysis. Sensors 2021, 21, 5769.

[3] Asadollahkhan Vali, A. (2022). Airport Pavement Management System: Assessing current condition and estimating remaining life from aircraft demand. Spectrum Research Repository.

How to cite: Tessema, T., Ardakanian, A., Bolton, M., Fairley, R., Karastamati, A., Smith, R., Fernandez, J., and Tosti, F.: Multi-modal Remote Sensing and in-situ Sensors Integration for Advanced Airport Asset Monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19237, https://doi.org/10.5194/egusphere-egu26-19237, 2026.

The conservation of ancient architectural heritage remains a fundamental and persistent challenge in cultural heritage management. Wall paintings constitute a significant component of this heritage, representing early and highly valuable forms of artistic expression, particularly within religious and historical buildings from major historical periods such as the Renaissance. Among these works, the mural paintings attributed to Giotto, the founder of modern Western painting and one of the most influential figures in Italian art history, are of outstanding cultural and historical significance.

With the passage of time, wall paintings are increasingly affected by physical and environmental degradation, making their systematic assessment and preservation a critical priority. The identification and characterization of subsurface deterioration within masonry walls and wall paintings, structures that are inherently fragile and multilayered, require the application of reliable non-destructive testing (NDT) techniques. Such deterioration may manifest as subsurface moisture accumulation, voids, or delamination between layers, often induced by environmental factors such as diurnal and seasonal temperature fluctuations, humidity variations, and anthropogenic influences.

Recent advancements in NDT technologies have enabled more detailed investigation of the internal structure of heritage materials.  Among these techniques, Ground Penetrating Radar (GPR) has emerged as a particularly effective tool due to its rapid data acquisition, cost-effectiveness compared to destructive methods, portability, and suitability for non-invasive time-lapse monitoring, as well as its capability to provide high-resolution two-dimensional and three-dimensional imaging of subsurface features. Despite its potential, the application of GPR to wall paintings remains limited, primarily due to challenges associated with data processing and interpretation in complex, thin-layered media [1, 2].

This study aims to address these limitations by developing and applying advanced GPR processing and interpretation strategies for improving the detection and characterization of subsurface defects and material heterogeneities within wall paintings. Considering the limited thickness of the plaster and painted layers, a 2 GHz GPR system with crossed polarized antennas was employed to maximize spatial resolution. Although the high operating frequency restricts penetration depth, it enables detailed imaging of near-surface features that are critical for the diagnostic assessment of wall paintings.

Keywords: Ground Penetrating Radar; Cultural Heritage; Wall Paintings; Non-Destructive Testing; Giotto

Acknowledgement: The authors would like to acknowledge the fruitful visiting scholar exchange between the University of West London (UWL) Faringdon Centre and the University of Florence, which significantly contributed to the successful completion of this study. Additionally, the authors would like to thank Dr. Maria Rosa Lanfranchi (OPD), the restorer, for the contribution to this work.

References

1. Napoli, A. F., Marchetti, E., Coli, M., Ciuffreda, A. L., Morandi, D., Papeschi, P., and Agostini, B.: Application of Ground Penetrating Radar (GPR) analysis on San Giovanni's Baptistery in Florence, EGU 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-12917, https://doi.org/10.5194/egusphere-egu24-12917.

2. Ortega-Ramirez, M. Bano, L. A. Villa Alvarado, D. Medellin Martinez, R. Rivero-Chong, C. L. Motolinia-Temol, High-resolution 3D GPR applied in the diagnostic of the detachment and cracks in pre-Hispanic mural paintings at “Templo Rojo,” Cacaxtla, Tlaxcala, Mexico. Journal of Cultural Heritage 50 (2021) 61-72, doi:https://doi.org/10.1016/j.culher.2021.06.008.

How to cite: Napoli, A. F., Parnow, S., Marchetti, E., and Tosti, F.: A High-resolution Ground-Penetrating Radar Framework for Detecting Subsurface Discontinuities in Historic Wall Paintings: A Case Study of Giotto's Mural Paintings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20938, https://doi.org/10.5194/egusphere-egu26-20938, 2026.

EGU26-21528 | ECS | Orals | GI5.2

Parametric prediction of GPR diffraction hyperbolas from top-down pavement cracks using gprMax FDTD simulations 

Grigório Neto, Francisco Fernandes, Simona Fontul, and Jorge Pais

Ground penetrating radar is used in asphalt pavement condition assessment due to rapid acquisition and sensitivity to dielectric contrasts. For top down cracking, interpretation often relies on diffraction hyperbolas, while the relation between crack geometry and measurable hyperbola descriptors is frequently handled by visual inspection. This study defines a parametric physics based workflow that links detected hyperbolas to crack depth ratio and crack aperture using gprMax forward simulations and automatic hyperbola parameter extraction.

Two dimensional finite difference time domain simulations are performed in gprMax for a layered pavement composed of an asphalt layer over a granular base. Electromagnetic properties are prescribed by relative permittivity and effective conductivity, using relative permittivity 5.50 and conductivity one times ten to the minus four siemens per metre for asphalt, and relative permittivity 6.00 and conductivity one times ten to the minus four siemens per metre for the granular layer. The parametric space includes asphalt thickness between 0.05 and 0.30 m, crack aperture from 2 to 20 mm, crack depth ratio between 0.20 and 1.00 of the asphalt thickness, and antenna central frequencies of 1.6 GHz and 2.3 GHz. Representative configurations are selected from the full combination space.

Synthetic B scans are processed by time zero correction, dewow filtering, background subtraction using trace mean removal, and repeated moving average smoothing. Peak candidates are identified on a central trace defined by the maximum absolute amplitude at an early time sample. Each candidate is tracked laterally by a local maximum search within a symmetric vertical window around the previous pick, yielding a set of points that describe the diffraction trajectory. Each trajectory is parameterised by fitting a quadratic time squared versus offset squared model, with the apex position set by the estimated trajectory centre. The fit provides the apex time, the curvature parameter, and the asymptote slope derived from the curvature. The maximum absolute amplitude along each trajectory is extracted as an amplitude indicator with its space time coordinates. Upper and lower trajectories are assigned by ordering apex times.

The workflow outputs a frequency and thickness conditioned mapping between crack geometry and paired hyperbola descriptors for the upper and lower trajectories, including apex times, curvature based parameters, asymptote slopes, and amplitude indicators. The prediction model is expressed as a conversion from the detected upper and lower hyperbola descriptors, conditioned on frequency, asphalt thickness, and prescribed material properties, to the crack depth ratio and crack aperture. This formulation answers the guiding question by providing an explicit link between measured hyperbola parameters and quantitative crack characteristics under controlled acquisition and material conditions.

How to cite: Neto, G., Fernandes, F., Fontul, S., and Pais, J.: Parametric prediction of GPR diffraction hyperbolas from top-down pavement cracks using gprMax FDTD simulations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21528, https://doi.org/10.5194/egusphere-egu26-21528, 2026.

EGU26-22638 | Orals | GI5.2

Regularized Inverse Near-Field Synthesis of Antenna Currents Using RWG Basis Functions 

Amitabha Bhattacharya and Ananya Dey

Inverse electromagnetic source problems are inherently ill-posed, as small perturbations in the measured or prescribed fields can lead to large variations in the reconstructed current distributions, necessitating appropriate regularization to suppress non-physical and superdirective solutions. In this work, an inverse Method of Moments (MoM) formulation [1] based on Rao–Wilton–Glisson (RWG) basis functions [2] are developed for near-field antenna pattern synthesis. The forward operator is constructed by mapping RWG surface current coefficients to the near electric field through a dipole-based radiation approximation, yielding a linear but severely ill-conditioned inverse problem.
The resulting inverse formulation is solved using Tikhonov regularization [3], which stabilizes the solution by balancing field fidelity against current smoothness. The regularization parameter is selected using the classical L-curve criterion [4], which is shown to provide a stable and physically meaningful trade-off between the residual norm and the solution norm for the proposed inverse MoM framework. Numerical results demonstrate accurate synthesis of a near-field sector beam spanning approximately ±60° in angle, with the synthesized IEyI distribution closely matching the prescribed field profile. The reconstructed RWG surface currents remain spatially smooth and bounded in magnitude, indicating effective suppression of non-physical and superdirective solutions.
The proposed approach offers a robust and computationally efficient framework for inverse near-field antenna synthesis using surface integral formulations, and provides a validated foundation for future extensions to electrically large structures, inverse antenna–metamaterial design, and more complex inverse radiation control problems.

 

Fig.1: L curve for obtaining an appropriate 𝜆

 

Fig.2: Synthesized surface current for sector pattern for 𝜃=60° at 𝜌=0.01𝜆

Fig.3: Comparison plot of desired and synthesized sector pattern for 𝜃=60° at 𝜌=0.01𝜆

 

References
[1] S. H. Raad, J. S. Meiguni, and R. Mittra, “Inverse MoM Approach to Near-Field Prediction and RFI Estimation in Electronic Devices With Multiple Radiating Elements,” IEEE Access, vol. 11, pp. 21313–21325, 2023.
[2] S. Rao, D. Wilton, and A. Glisson, “Electromagnetic Scattering by Surfaces of Arbitrary Shape,” IEEE Transactions on Antennas and Propagation, vol. 30, no. 3, pp. 409–418, 1982.
[3] D.-H. Han, X.-C. Wei, D. Wang, W.-T. Liang, T.-H. Song, and R. X. K. Gao, “A Phase less Source Reconstruction Method Based on Hybrid Dynamic Differential Evolution With Least Square and Regularization,” IEEE Transactions on Electromagnetic Compatibility, vol. 66, no. 2, pp. 566–573, 2024.
[4] P. C. Hansen, “The L-curve and its use in the numerical treatment of inverse problems,” SIAM Review, vol. 34, no. 4, pp. 561–580, 1992.

How to cite: Bhattacharya, A. and Dey, A.: Regularized Inverse Near-Field Synthesis of Antenna Currents Using RWG Basis Functions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22638, https://doi.org/10.5194/egusphere-egu26-22638, 2026.

EGU26-22982 | ECS | Posters on site | GI5.2

From Detection to Interpretation: A Decision-Support Framework for GPR-Based Evidence in Urban Climate Adaptation 

Livia Lantini, Atiyeh Ardakanian, and Fabio Tosti

Urban climate adaptation strategies increasingly rely on trees as multifunctional assets for mitigating heat stress and improving urban liveability [1]. As tree planting and management accelerate in response to climate pressures, interactions between urban trees and subsurface infrastructure become increasingly relevant for planners, asset managers, and local authorities operating at neighbourhood to asset-management scales. Ground Penetrating Radar (GPR) is a well-established non-destructive technique for imaging shallow subsurface conditions and detecting tree root systems in urban environments [2], yet its contribution to adaptation-oriented decision contexts remains limited.

This limitation is not necessarily related to detection capability, as in some instances this depends on how GPR outputs are transformed and communicated beyond individual case studies. In climate adaptation settings, decisions concerning tree retention, monitoring, and intervention typically rely on surface-based indicators and qualitative risk categories [3], limiting the use of subsurface information for cross-site comparison and prioritisation within decision-support processes.

To address this gap, GPR data from multiple urban sites within the same local area were analysed to capture subsurface conditions around urban trees and their interaction with pavements and engineered layers. Rather than focusing on site-specific detection outcomes, the methodology introduced an intermediate analytical step in which GPR profiles were structured into repeatable spatial units and used to derive relative, non-prescriptive descriptors of subsurface conditions. These descriptors were explored through alternative indicator formulations, allowing different representations of subsurface variability and uncertainty to be examined while remaining grounded in the same geophysical observations. Within this framework, the resulting indicators were then synthesised at tree level to support decision-relevant interpretation, enabling subsurface conditions to be characterised in comparative terms and translated into high-level management tendencies, such as prioritisation for monitoring, further investigation, or intervention.

The study demonstrates that reframing GPR outputs within a stakeholder-oriented decision-support framework, rather than site-specific detection outcomes, enhances their relevance for climate adaptation and resilience planning. The proposed approach provides a transferable pathway for integrating geophysical evidence into evidence-based urban policy and asset management processes, by explicitly aligning geophysical interpretation with the scale and needs of real-world decision-making.

 

Keywords: Ground Penetrating Radar (GPR); Urban Trees; Decision-support Framework; Urban Resilience; Climate Adaptation

 

References

[1] D.E. Bowler, L. Buyung-Ali, T.M. Knight and A.S. Pullin, "Urban greening to cool towns and cities: A systematic review of the empirical evidence," Landscape and Urban Planning, vol. 97, pp. 147–155, Sep 15. 2010.

[2] L. Lantini, F. Tosti, I. Giannakis, L. Zou, A. Benedetto and A.M. Alani, "An Enhanced Data Processing Framework for Mapping Tree Root Systems Using Ground Penetrating Radar," Remote Sensing, vol. 12, pp. 3417, Oct 1. 2020.

[3] S. Pauleit, T. Zölch, R. Hansen, T.B. Randrup and C. Konijnendijk van den Bosch, "Nature-Based Solutions and Climate Change – Four Shades of Green," in Nature-Based Solutions to Climate Change Adaptation in Urban Areas: Linkages between Science, Policy and Practice, N. Kabish, H. Korn, J. Stadler and A. Bonn, Springer, 2017, pp. 29–50.

How to cite: Lantini, L., Ardakanian, A., and Tosti, F.: From Detection to Interpretation: A Decision-Support Framework for GPR-Based Evidence in Urban Climate Adaptation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22982, https://doi.org/10.5194/egusphere-egu26-22982, 2026.

EGU26-23142 | ECS | Orals | GI5.2

Rebar corrosion assessment using polarimetric ground penetrating radar 

Bin Zhang, Hai Liu, Pei Wu, and Xu Meng

Ground Penetrating Radar (GPR) has been widely used for non-destructive testing to detect reinforcing bars (rebars) in concrete. However, the mechanism-level interpretation and quantitative characterization of GPR responses from corroded rebars remain at an early stage. Existing single-polarization GPR approaches mainly rely on echo amplitude and time-delay features to infer corrosion, yet these responses are highly sensitive to experimental conditions and environmental factors, leading to inconsistent trends [1]. With the advancement of polarimetric GPR, increasing attention has been paid to leveraging polarization information for rebar corrosion detection [2]. Nevertheless, existing polarimetric power decomposition methods often classify rebar returns as being dominated by surface scattering, whereas rebars exhibit a typical linear geometry and should theoretically present a pronounced dipole-scattering component.

To address this issue, we propose a four-component polarimetric decomposition method for rebar scattering characterization and corrosion-state evaluation. Building upon the Dey three-component decomposition [3] and inspired by the Huynen decomposition [4], the proposed method uses the real part of T12, i.e.,  R{T12} as a key indicator of dipole scattering. This term can be interpreted as a shape-related indicator that tends to be pronounced for line-like targets, enabling a physically interpretable decomposition of the total scattering power into four components: surface scattering, double-bounce scattering, volume scattering, and dipole scattering.

Experiments were conducted using a VNA-based full-polarimetric GPR system equipped with dual-polarized Vivaldi antennas operating from 0.7 to 6 GHz. Reinforced concrete specimens with a 12 mm diameter rebar and a 50 mm concrete cover were tested under an indoor accelerated corrosion setup over 20 days. For each corrosion day, the scattering powers of the four components were computed and normalized, and the mean values were extracted within a region of interest (ROI) centered on the rebar response. The decomposition results indicate that the rebar scattering is primarily governed by dipole and surface scattering. Moreover, the temporal evolution of the decomposed powers over the corrosion period reveals that the dipole scattering power is more sensitive to corrosion progression than the surface scattering component, suggesting it as an effective feature for evaluating corrosion stage and tracking corrosion development.

References

[1] Faris N, Zayed T, Abdelkader E M, et al. Corrosion assessment using ground penetrating radar in reinforced concrete structures: Influential factors and analysis methods[J]. Automation in Construction, 2023, 156: 105130.

[2] Liu H, Zhong J, Ding F, et al. Detection of early-stage rebar corrosion using a polarimetric ground penetrating radar system[J]. Construction and Building Materials, 2022, 317: 125768.

[3] Dey S, Bhattacharya A, Ratha D, et al. Target Characterization and Scattering Power Decomposition for Full and Compact Polarimetric SAR Data[J]. IEEE Transactions on Geoscience and Remote Sensing, 2021, 59(5): 3981-3998. DOI:10.1109/TGRS.2020.3010840.

[4] Huynen J R. Stokes matrix parameters and their interpretation in terms of physical target properties[C]//Polarimetry: Radar, infrared, visible, ultraviolet, and X-ray. SPIE, 1990, 1317: 195-207.

How to cite: Zhang, B., Liu, H., Wu, P., and Meng, X.: Rebar corrosion assessment using polarimetric ground penetrating radar, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23142, https://doi.org/10.5194/egusphere-egu26-23142, 2026.

EGU26-1632 | ECS | Posters on site | GM2.6

Interplay Between Event Frequency and Intensity in Future Rainfall Erosivity revealed by Convection-permitting climate models 

Assumpta Ezeaba, Eleonora Dallan, Petr Vohnicky, and Marco Borga

Authors:

Ezeaba Assumpta1, Dallan Eleonora1, Vohnicky Petr1, Borga Marco1

1 Department of Land, Environment, Agriculture and Forestry, University of Padova, Legnaro, Italy

Type of presentation:

Poster

 

Title:

Interplay Between Event Frequency and Intensity in Future Rainfall Erosivity revealed by Convection-permitting climate models

 

Abstract:

Soil erosion represents a critical environmental and economic challenge facing agricultural landscapes, and its severity could be amplified by the rising intensity of extreme rainfall in a warming climate. Rainfall erosivity, a key driver of erosion, depends on both rainfall intensity and the frequency of erosive events, making it highly sensitive to their ongoing and future changes. High resolution convection-permitting models (CPMs) offer enhanced representation of sub-daily rainfall extremes, yet their application to soil erosion studies remains limited.

This work assesses the skill of an hourly CPM in reproducing historical rainfall erosivity in a Mediterranean Island, Sicily, and evaluates its future changes under RCP4.5 and RCP8.5 scenarios. Modelled rainfall was first bias-corrected using intensity thresholds and scaling factors derived from high temporal-resolution observations. The CPM shows underestimate in maximum rainfall intensity and erosive event frequency, and thus in mean annual erosivity, especially in lowland and coastal areas. These biases highlight challenges in simulating short-duration convective events, sea-land interactions, and mismatches between point-based and gridded datasets. Future projections show divergent outcomes: under RCP4.5 moderate frequency decrease combines with higher intensities leading to a moderate net increase in erosivity, whereas under the RCP8.5 scenario a marked (17%) reduction in event frequency dominates the signal, yielding lower future erosivity despite rainfall intensification.

The results demonstrate that bias correction procedures should consider topographic dependence and different erosivity-related variables, and that future erosivity cannot be inferred from intensity changes alone; event frequency is equally relevant. Incorporating high-resolution climatic models and explicitly accounting for frequency-intensity interactions are therefore essential for robust erosion risk assessments and climate adaptation strategies.

 

This study was carried out within the RETURN Extended Partnership and received funding from the European Union Next‐GenerationEU (National Recovery and Resilience Plan—NRRP, Mission 4, Component 2, Investment 1.3—D.D. 1243 2/8/2022, PE0000005); and within the Space It Up project funded by the Italian Space Agency, ASI, and the Ministry of University and Research, MUR, under contract n. 2024-5-E.0 - CUP n. I53D24000060005.

How to cite: Ezeaba, A., Dallan, E., Vohnicky, P., and Borga, M.: Interplay Between Event Frequency and Intensity in Future Rainfall Erosivity revealed by Convection-permitting climate models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1632, https://doi.org/10.5194/egusphere-egu26-1632, 2026.

EGU26-2481 | Orals | GM2.6

A Fully-Resolved Simulation Study of Seabed Liquefaction and Dynamic Response Using a Coupled LBM-IBM-DEM Approach 

Jinfeng Zhang, qinghe Zhang, zhongyue Li, and guangwei Liu

Wave-induced seabed liquefaction is a common factor leading to submarine instability, primarily occurring in silty seabeds. Under wave action, the pore water pressure within the seabed continuously increases. When the pore water pressure approaches or exceeds the total stress of the soil, the effective stress of the soil tends toward zero, resulting in liquefaction. Currently, most models of seabed dynamic response are based on macroscopic constitutive equations derived from Biot’s consolidation theory, making it difficult to accurately reveal the mesoscale mechanisms of seabed behavior under wave loading. This study employs a coupled numerical approach integrating the Lattice Boltzmann Method (LBM), the Immersed Boundary Method (IBM), and the Discrete Element Method (DEM) to systematically investigate the dynamic response and liquefaction process of a seabed under wave action. In this model, DEM is used to describe the motion and interactions of seabed sediment particles, LBM is applied to simulate fluid flow behavior, and IBM handles the coupling effects between particles and the fluid. Additionally, to improve computational efficiency, local grid refinement is applied near the seabed region, enhancing overall calculation performance. Using this coupled model, the periodic variations of wave-induced pore water pressure and effective stress in the seabed are studied, and the simulation results are validated against experimental data. The results show good agreement between simulations and experiments, accurately reflecting the dynamic response characteristics of the seabed under wave action. The model not only reveals the interaction mechanisms between soil particles and pore fluid from a microscopic perspective but can also be further extended to study the coupled effects of liquefaction and scour on near-bed sediment transport, offering significant theoretical insights and practical engineering value.

How to cite: Zhang, J., Zhang, Q., Li, Z., and Liu, G.: A Fully-Resolved Simulation Study of Seabed Liquefaction and Dynamic Response Using a Coupled LBM-IBM-DEM Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2481, https://doi.org/10.5194/egusphere-egu26-2481, 2026.

There are no theoretical formulas that can accurately predict the sand transport rate (Qm) over the Gobi surface. We report herein high-frequency field observations of wind-blown sand processes over the Gobi surface under extremely high winds in eastern Xinjiang, China. The results reveal that the power-law exponent of the scaling relationship between Qₘ and friction wind velocity (uτ) in the extremely high winds with high gravel coverage Gobi area can reach 15.51, significantly exceeding that on sandy surfaces. Meanwhile, there is a favorable power-law between Qm and the fluctuation intensity of the vertical wind velocity (Iw), whereas the correlation between Qₘ and the streamwise fluctuation intensity (Iu) is weak. Therefore, Iw has a significant application in constructing the prediction model for Qₘ over such Gobi surfaces. This study provides a new insight into the quantitative analysis of the aeolian transport over the windy Gobi areas.

How to cite: Wang, T.: Sand Transport Rate and Turbulent Fluctuation in AeolianTransportation Over the Gobi Surface Under ExtremelyHigh Winds, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2690, https://doi.org/10.5194/egusphere-egu26-2690, 2026.

EGU26-2920 | Orals | GM2.6

Debris Flow Surges Amplification Controlled by Topography and Rheology 

Dongri Song and Yunhui Liu

Field observations in the Jiangjia Ravine show that surge characteristics evolve systematically along the flow path. As the flows transition from steep upstream slopes to gentler downstream reaches, surge forms shift from high-frequency low-amplitude surges to low-frequency high-amplitude surges. To explain the spatial evolution of surges, we develop a mechanistic model governed by slope geometry and yield stress. The shear stress can fall below the yield stress at slope breaks, temporarily blocking the flow. Subsequent surges with higher shear stress exceed the yield stress and remobilize the stored material. Experimental results show that on the steep slope, the mixture generates unsteady roll waves. Once these waves reach the gentle slope, they further amplify and evolve into distinct surge fronts, confirming the proposed model. These findings establish a conceptual framework for understanding the accelerated evolution of debris-flow surges.

How to cite: Song, D. and Liu, Y.: Debris Flow Surges Amplification Controlled by Topography and Rheology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2920, https://doi.org/10.5194/egusphere-egu26-2920, 2026.

Extreme hydro-meteorological events are among the primary drivers of hydrologic and geomorphic hazards, posing an increasing threat to societies worldwide. The combined effects of climate change, and increased exposure and vulnerability in hazard-prone areas have led to a continuous rise in disaster risk.
This contribution addresses some key challenges in forecasting and managing hydro-meteorological processes across two main interrelated contexts—data-rich or data-scarce regions—which, despite their known differences, share common issues of scale, complexity, and uncertainty in hazard–society interactions.
In both environments, local-scale factors such as small-scale processes, and human disturbances interact with regional climate variability and large-scale atmospheric drivers to shape evolving hydro-geomorphic processes. At the same time, decisions happen at national, basin, or urban scales, often creating cross-scale mismatches between where hydro-meteorological processes materialize and where decisions are taken.
The presentation discusses how Earthcasting-oriented approaches, such as the integration of remote sensing, reanalysis products, crowd-sourced information, and qualitative socio-economic data, can partially address these gaps. While these data sources introduce new uncertainties, they also provide opportunities to improve awareness and support process-based forecasts and decision-making in regions where conventional data are unavailable, or they might not be enough.
Building on recent advances in technology but also risk science, this talk advocates for integrated assessment frameworks that explicitly account for cross-scale interactions, feedbacks, and data limitations, also highlighting implications for communication strategies. Ultimately, advancing such integrated approaches is essential for translating scientific knowledge into an added social value of the predictability of Earth surface processes.

How to cite: Sofia, G.: From Climate Data to Decisions in the Age of Extremes:  Challenges and Opportunities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3013, https://doi.org/10.5194/egusphere-egu26-3013, 2026.

EGU26-4395 | ECS | Posters on site | GM2.6

An Evaluation of Riverbed Roughness Metrics Derived from UAV–SfM Point Clouds and Their Relationships with Grain Size Distribution in Mountain Rivers 

Tung Yang Lai, Chyan Deng Jan, Kuan Chung Lai, and Yu Chao Hsu

Understanding sediment grain size distribution in riverbeds is fundamental to analyses of sediment transport, riverbed morphology, and ecological habitats. Recent advances in unmanned aerial vehicle (UAV)–Structure-from-Motion (SfM) photogrammetry have enabled indirect characterization of sediment grain size (D) using surface roughness (R) derived from point cloud analyses. However, the relationships between grain size and roughness, as obtained using different roughness metrics in mountain rivers, remain insufficiently investigated.

In this study, manual sediment sampling and high-resolution UAV surveys were conducted across multiple mountainous river reaches in Taiwan, characterized by coarse bed materials and wide grain size distributions. SfM-derived point clouds were used to compute three roughness metrics: roughness height (RH), standard deviation of elevations (σ), and detrended standard deviation (σd). Linear relationships were established between local grain sizes (Di, where i = 16, 25, 50, 75, and 84) and their corresponding percentile roughness values (Ri). In addition, integrated power-law relationships were developed by pooling all paired Di–Ri data across the study reaches.

The results indicate that all three roughness metrics (RH, σ, and σd) exhibit strong correlations with grain size in gravel-bed rivers when analyses are conducted within the same river reach. The linear Di–Ri relationships show moderate to strong correlations (R² = 0.57–0.95), with the D50–R50 relationship demonstrating the highest consistency across all three metrics. Similarly, the integrated power-law relationships derived from the three roughness metrics yield high correlations (R² = 0.89–0.93). However, notable differences emerge when these relationships are applied to other river reaches. The RH-based relationship maintains more consistent predictive performance, whereas relationships derived from σ and σd exhibit larger deviations. These results suggest that RH-based roughness metrics offer superior applicability for estimating sediment grain size in mountain rivers. Overall, this study provides practical insights into the selection of suitable roughness metrics for grain size estimation in coarse-grained riverbeds.

How to cite: Lai, T. Y., Jan, C. D., Lai, K. C., and Hsu, Y. C.: An Evaluation of Riverbed Roughness Metrics Derived from UAV–SfM Point Clouds and Their Relationships with Grain Size Distribution in Mountain Rivers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4395, https://doi.org/10.5194/egusphere-egu26-4395, 2026.

EGU26-5017 | Orals | GM2.6

A depth-averaged grain-fluid model with dilatancy and an upper-solid layer 

Anne Mangeney, Francois Bouchut, Enrique Fernandez-Nieto, and Gladys Narbona-Reina

To effectively assess the growing hazard related to debris flows, it is crucial to simulate these natural
grain-fluid flows at a reasonable computational cost. To complement existing depth-averaged grain-fluid flow
models with an upper-fluid layer, we propose here a model with an upper-solid layer, as a first step towards the
development of unified models describing all possible configurations. This model accounts for granular mass
dilatancy and pore fluid pressure feedback and solves for solid and fluid velocity in the mixture and for the
upper-solid velocity. Simulation in uniform configurations reveals the rich behaviour of the flow and shows that
the upper-solid and upper-fluid models may predict very different behaviour. Our work highlights the need of
developing two-layer models accounting for dilatancy and unifying upper-solid and upper-fluid configurations
in the same framework.

How to cite: Mangeney, A., Bouchut, F., Fernandez-Nieto, E., and Narbona-Reina, G.: A depth-averaged grain-fluid model with dilatancy and an upper-solid layer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5017, https://doi.org/10.5194/egusphere-egu26-5017, 2026.

EGU26-5469 | ECS | Orals | GM2.6

Semi-resolved LES–DEM simulations of turbulent bedload transport from saltation to sheet flow regimes 

Yuxiang Liu, Lu Jing, Zi Wu, and Xudong Fu

Bedload transport is ubiquitous in natural environments and encompasses flow regimes from saltation to sheet-flow, characterized by distinct fluid–particle interaction mechanisms. Accurately capturing these processes requires a numerical approach that can capture both turbulence and fluid-particle interactions, for which challenges exist due to the constraints of grid resolution on the coupling accuracy. In this study, we propose a semi-resolved LES–DEM framework to overcome such limitations in the conventional CFD-DEM paradigm. A feedback-controlled body-force term is also proposed to maintain a prescribed discharge under periodic boundary conditions in turbulent open-channel flow simulations. Three benchmark cases are conducted to assess the accuracy and robustness of the proposed framework, including clear-water turbulent channel flow as well as bedload transport in both saltation and sheet-flow regimes. The present method is demonstrated to effectively overcome the conventional grid-size limitation and thus allows the fluid field to be resolved on sufficiently fine grids while preserving accurate fluid-particle coupling. We further investigate the micromechanical processes underlying the transition from the saltation to sheet-flow regimes and quantify the thickness of the transport layers as functions of the Shields number. Overall, this framework provides a unified and reliable numerical tool for simulating sediment transport across a broad range of flow regimes, offering a solid basis for micromechanical analysis and the development of continuum models.

How to cite: Liu, Y., Jing, L., Wu, Z., and Fu, X.: Semi-resolved LES–DEM simulations of turbulent bedload transport from saltation to sheet flow regimes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5469, https://doi.org/10.5194/egusphere-egu26-5469, 2026.

EGU26-7103 | ECS | Orals | GM2.6

Size segregation of granular mixtures under recirculation 

Yanan Chen and Christophe Ancey

Particle-size segregation is a common phenomenon in granular materials that has attracted increasing attention in recent years. Yet segregation under recirculation remains underexplored compared to segregation in simple-sheared gravity-driven flows. In this study, we investigated the dynamics of a bi-dispersed granular mixture flowing over an inclined conveyor belt. This belt pulled particles upstream, creating a recirculating flow. We visualized the internal structure of granular flow in a vertical plane by matching the refractive indices of the fluid and particles, and then located the particles. We observed an upstream accumulation of small particles and downstream accumulation of large particles, these two regions being separated by a curved interface. We think that this separation resulted from the interplay between particle recirculation and segregation: 1) surface particles moved downstream while bottom particles moved upstream; 2) segregation led to particles separating during recirculation, with full separation achieved at the channel ends. We developed a depth-averaged advection-diffusion equation to quantify this phenomenon by treating the recirculation as convection. This study provides new insights into the coupled mechanisms of recirculation and segregation in granular materials.

How to cite: Chen, Y. and Ancey, C.: Size segregation of granular mixtures under recirculation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7103, https://doi.org/10.5194/egusphere-egu26-7103, 2026.

EGU26-7135 | ECS | Orals | GM2.6

Fluvial geomorphology and historical evolution of the Var River, France: a case study of a highly anthropic Mediterranean braided channel 

Sebastián Granados-Bolaños, Fanny Picourlat, Youness Ouassanouan, Felix Billaud, Margot Chapuis, and Morgan Abily

The Var River in southeastern France represents an example of a Mediterranean fluvial system profoundly modified by human activity. Over the past eight decades, engineering works, gravel mining, and urbanization have progressively confined and simplified the channel, while the river remains a vital water resource for the city of Nice and its surroundings.

We present a multi-temporal and multi-scale analysis of the lower Var River’s morphological evolution between 1940 and 2025. Historical aerial and satellite images (n > 50) were analyzed to quantify changes in braided index, channel confinement ratio, slope–width relationships, and channel morphology classes. A high-resolution UAV survey conducted in 2025 covered 20 km of the lower valley, producing detailed orthomosaics and digital elevation models from over 80,000 images. Additional sedimentological analyses combining terrestrial photogrammetry and laboratory measurements thoroughfully characterized grain size and lithology of fluvial landforms.

Results reveal a complex spatial pattern in channel form: the lower Var alternates between multi-thread and single-thread morphologies along its 20 km course, with transitions occurring over distances of less than one km. These abrupt shifts are linked to local confinement, engineered structures (among which weirs which underwent recent lowering), and bedload disconnection. Overall, the river has undergone strong simplification and narrowing, with active-channel reductions exceeding 60% in channelized reaches. The present morphology reflects a hybrid, fluvial state shaped by human regulation and contrasted hydrology. These findings provide new insights into the geomorphic resilience of Mediterranean rivers and inform sediment management and corridor planning for the Nice Metropolitan region, since it present the first high-resolution analysis of this fluvial corridor.

How to cite: Granados-Bolaños, S., Picourlat, F., Ouassanouan, Y., Billaud, F., Chapuis, M., and Abily, M.: Fluvial geomorphology and historical evolution of the Var River, France: a case study of a highly anthropic Mediterranean braided channel, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7135, https://doi.org/10.5194/egusphere-egu26-7135, 2026.

Granular sediments in rivers, coasts, and pipelines often undergo particle size segregation due to the action of the carrier fluid and particle-particle interactions. This process can significantly affect geomorphology and the associated geohazards, but our mechanistic understanding of granular segregation in fluid-driven bedload transport remains elusive. In this study, a particle-scale numerical simulation based on the coupled computational fluid dynamics–discrete element method (CFD-DEM) is conducted to investigate the segregation of a bidisperse bed sheared by high-viscosity fluids. The evolution of segregation under varying shear intensities, characterized by the Shields number, is systematically analyzed in laminar flow. The results show that: (1) under various Shields numbers, the granular bed can be divided into an upper bedload layer (fluid-like, fast-moving) and a lower creep layer (solid-like, slowly moving), with the bedload layer thickening and the creep layer thinning linearly as the shear intensity increases; (2) particle segregation evolves exponentially over time, and at the same duration, the final degree of segregation for the entire bed increases linearly with the Shields number; (3) the segregation timescale shows a non-monotonic dependence on the Shields number, governed by the competing effects of increasing segregation velocity and active layer thickness as the Shields number is increased; and (4) the segregation timescale follows a power-law relationship with the shear rate in laminar flow, showing similarities to dry granular flow behavior. Future work will focus on developing a predictive model that captures the evolution of coarse and fine particle concentration profiles, thereby enhancing our modeling capabilities of granular segregation and its feedback effects on the mobility of sediment transport.

How to cite: Li, X. and Jing, L.: Size Segregation of Bidisperse Granular Beds in Laminar Shear Flow: A CFD-DEM Investigation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8573, https://doi.org/10.5194/egusphere-egu26-8573, 2026.

EGU26-9692 | ECS | Posters on site | GM2.6

Evaluation of a downscaled Regional Climate Model for analysing the frequency of debris flows since 1850 

Jakob Rom, Madlene Pfeiffer, Ben Marzeion, Tobias Heckmann, Florian Haas, and Michael Becht

Debris flows are a major natural hazard in mountainous regions worldwide and significantly impact the sediment budgets in alpine areas. However, the development of debris flow frequency under climate change conditions has not yet been conclusively clarified, as long-term, comprehensive event records (i.e. not biased towards large events) are scarce. As alpine debris flows are predominantly triggered by high-intensity and short-duration rainfall events, precipitation records can be useful for inferring potential triggers, particularly under transport-limited conditions. As high-resolution precipitation measurements are rarely available over long periods of time, we employed dynamical downscaling of a Regional Climate Model (RCM) based on the Advanced Weather Research and Forecasting model (WRF). This approach resulted in a high-resolution climate model dataset covering most of the Central Alps, with a spatial resolution of 2x2 km and a temporal resolution of 15 minutes. This model enabled us to analyse high-intensity, short-duration rainfall events since the end of the Little Ice Age in 1850.

We compared the RCM with a debris flow record in the Horlachtal catchment in Tyrol, Austria. By analysing remote sensing datasets such as historical and recent aerial imagery, airborne lidar data and lichenometric dates, we identified 991 individual debris flows in the area between 1947 and 2022. Combining the observation dataset with the RCM rainfall data enabled us to take an integrated approach to assessing changes in debris flow frequency in the Horlachtal and their climatic drivers since 1850. The results provide insights into possible future trends in debris flow frequency in a changing climate, showing a weak positive long-term trend for the Horlachtal. The RCM's coverage allows for similar studies in other Alpine regions, offering more detailed insights into the spatial variability of changes in debris flow activity within the Central Alps.

How to cite: Rom, J., Pfeiffer, M., Marzeion, B., Heckmann, T., Haas, F., and Becht, M.: Evaluation of a downscaled Regional Climate Model for analysing the frequency of debris flows since 1850, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9692, https://doi.org/10.5194/egusphere-egu26-9692, 2026.

EGU26-9737 | ECS | Orals | GM2.6

Morphodynamic responses to the 2000 Yigong dam-break flood: Insights from back-analysis and cross-scale modelling challenges 

Yunlong Lei, Marwan Hassan, Giorgio Rosatti, Luigi Fraccarollo, Daniel Zugliani, Xudong Fu, and Hongling Shi

Landslide Dam-Break Outburst Floods (LDBOF) are devastating natural hazards that drastically reshape downstream river morphologies. However, their inaccessibility, high risk of equipment loss, and sparse field data collection severely hinder hazard understanding and timely warning capabilities. The 2000 Yigong LDBOF event in China is one of the most significant modern recorded cases, yet it suffers from limited observational data. To address this gap, we integrated multi-source data—including open-source elevation datasets, literature-derived records, satellite-based flood inundation extents, and direct field observations—to develop a comprehensive input dataset for hydro-morphodynamic modeling of the event. Model validation against field observations and comparable studies confirmed the reasonableness of simulated lake emptying, dam breaching, flood inundation, bank erosion, and channel infilling processes. Our results reveal key morphodynamic characteristics of the Yigong LDBOF: dam material transport was dominated by translational motion during the flood rising stage and dispersive transport during the falling stage. The outburst flood peak discharge reached ~60 times that of typical meteorological floods, significantly amplifying the effects of river width on dam material transport. We further proposed a sediment transport equation that incorporates the regulatory effect of large boulders. Post-event channel recovery simulations, validated with remote sensing data, indicated minimal planform changes, with bed incision driven by headward erosion as the dominant morphological adjustment. Large boulders acted as a stabilizing factor, limiting upstream erosion and forming sediment supply-limited reaches. This study provides a robust multi-source data integration and modeling framework for LDBOF events with sparse observations, offers new insights into cross-scale hydro-morphodynamic processes of extreme floods, and the proposed sediment transport equation improves the accuracy of simulating boulder-influenced sediment dynamics—supporting hazard risk assessment and downstream river management for future LDBOF events.

How to cite: Lei, Y., Hassan, M., Rosatti, G., Fraccarollo, L., Zugliani, D., Fu, X., and Shi, H.: Morphodynamic responses to the 2000 Yigong dam-break flood: Insights from back-analysis and cross-scale modelling challenges, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9737, https://doi.org/10.5194/egusphere-egu26-9737, 2026.

EGU26-11152 | ECS | Posters on site | GM2.6

Efficient Hydrodynamic Modeling at the Landscape Scale: Quantifying River Width and Shear Stress Variability to Decode Tectonic Signals 

Boris Gailleton, Philippe Steer, Guillaume Cordonnier, and Fiona Clubb

Basal shear stresses exerted by river flow control the capacity of river to erode and transport sediment. Material properties (e.g. lithology, grain size) modulate how basal shear stress translates into morphological change. Quantifying the spatial variability of basal shear stress is therefore essential to assess fluvial erosion processes and to infer the tectonic and climatic forcings recorded in landscape morphology. 

Direct and systematic measurement of the basal shear stress in rivers is not feasible at large scales, making numerical hydrodynamic modelling the primary tool for its estimation. However, applications beyond the reach scale remain computationally prohibitive due to (i) the need for high-resolution topography to resolve channels, banks, and bars, and (ii) the numerical cost of solving the Shallow Water Equations (SWEs), which require small time steps to propagate changes induced and complex solvers. 

Here, we present a novel numerical framework that substantially reduces the computational cost of hydrodynamic modelling for morphometric analysis, enabling simulations over large, high-resolution DEMs and ranges of hydrological conditions. The approach reformulates the SWEs into a simplified stationary scheme, linearizing algorithmic complexity, and allowing scalable computations. In addition, we employ GPU-accelerated, graph-based flow accumulation algorithms to compute discharge efficiently. Together, these developments reduce computation time by up to three orders of magnitude compared to conventional hydraulic modelling approaches. 

The method is implemented in the pyfastflow package within the TopoToolbox ecosystem. We apply it to more than 100 watersheds in the Mendocino Triple Junction (California, USA), a region characterized by strong spatial gradients in tectonic uplift. Hydrodynamics are computed for five hydrological states constrained by precipitation data, spanning low flow to flood conditions. We quantify spatial variations in river width and shear stress and show that these metrics capture complementary temporal signatures of uplift timing and magnitude. Basin-wide shear stress responds quickly to uplift onset but exhibits a significantly delayed response during relaxation, whereas channel width displays a more variable and spatially contrasted transient signal upstream of the onset. 

How to cite: Gailleton, B., Steer, P., Cordonnier, G., and Clubb, F.: Efficient Hydrodynamic Modeling at the Landscape Scale: Quantifying River Width and Shear Stress Variability to Decode Tectonic Signals, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11152, https://doi.org/10.5194/egusphere-egu26-11152, 2026.

Coherent, energetic airflow structures control the incipient aeolian entrainment of coarse sediment and plastic debris, but their effect is poorly captured by classical, time-averaged shear-stress thresholds. This contribution showcases the results from recently published work [1, 2] that combines a particle-scale energy framework with wind-tunnel observations to quantify how individual sweeps and related structures trigger rocking, creep and full rolling, thereby regulating geomorphic work and debris mobility at Earth’s surface.

Wind-tunnel experiments were conducted in a 30 m environmental facility over a fixed rough bed of identical 40 mm celluloid spheres, representing idealized gravel and light plastic debris under fully turbulent, near-threshold flow (U ≈ 7.5–8.2 m s⁻¹). Synchronous 1 kHz measurements of near-bed airflow (2D hot-film) and particle displacement (0.1 mm laser distance sensor) resolve intermittent rocking and episodic rolling of a single exposed particle on a regular bed, under an atmospheric boundary layer with logarithmic mean profile and near-surface turbulence intensities up to ~20%.

A micromechanical model defines “energetic airflow events” as intervals where instantaneous drag exceeds an initial resistance level and persists for a finite duration, and relates their energy content Ef ∝ ∫u³dt to the minimum mechanical work F_g z_cr required to push a particle over its micro-topographic barrier. The resulting work-based criterion C_eff∫u³dt ≥ const introduces a normalized efficiency C_eff, estimated from the ratio of drag work ∫u²vdt to event energy, which partitions motion regimes from creep through rocking to incipient rolling and near-saltation. Quadrant analysis of uw shows that >85% of both rocking and rolling events are associated with Q4 sweeps; a simple peak-force condition u²_f,p ≥ u²_cr,0 is necessary for motion but insufficient for full entrainment, whereas the energy criterion correctly classifies ≈90–95% of observed rocking vs. rolling events. These results provide a transferable, event-based description of how coherent turbulent structures drive low-mobility aeolian transport, including mechanical sieving on gravel-mantled megaripples and the mobilisation of meso- to micro-plastic debris.

 

References

[1] Valyrakis, M., Zhao, X., Pähtz, T., & Li, Z. (2025). The role of energetic flow structures on the aeolian transport of sediment and plastic debris. Acta Mechanica Sinica, 41(1), 324467. https://doi.org/10.1007/s10409-024-24467-x.
[2] Zhao, X. H., Valyrakis, M., Pähtz, T., & Li, Z. S. (2024). The role of coherent airflow structures on the incipient aeolian entrainment of coarse particles. Journal of Geophysical Research: Earth Surface, 129(5), e2023JF007420. https://doi.org/10.1029/2023JF007420.

How to cite: Valyrakis, M., Pähtz, T., and Zhao, X.: From sweeps to sieving: a particle scale work-based criterion for intermittent aeolian entrainment of gravel and plastics under coherent turbulent structures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11556, https://doi.org/10.5194/egusphere-egu26-11556, 2026.

EGU26-11632 | ECS | Posters on site | GM2.6

 Influence of Pocket Geometry on the Incipient Entrainment of Coarse Particles in Turbulent Flows  

Aikaterini Papadaki and Manousos Valyrakis

The incipient motion of coarse particles critically governs bed stability, sediment transport dynamics, and geomorphic evolution in turbulent flows, with profound implications for riverbed destabilization, flood risk, and the integrity of hydraulic infrastructure. Despite extensive research, the ways under which microtopographic pocket arrangements—clusters or depressions formed by particle packing— modulate entrainment thresholds remains relatively underexplored. 
This presentation aims to outline the effects of varied pocket configurations on the critical hydraulic conditions required for particle entrainment under turbulent flow fields. Utilizing instrumented particles equipped with inertial measurement units (IMUs) [1, 2] to record high-fidelity particle accelerations and angular velocities, we probe both particle kinematics and dynamics, at the onset of motion. Novel flow-particle interaction metrics, derived from these measurements, reveal the underlying physical mechanisms—such as torque imbalances and lift generation—that drive or resist entrainment.
We hypothesize that subtle differences in pocket geometry and orientation can substantially elevate or lower the entrainment threshold, necessitating distinct flow field characteristics (e.g., shear stress and turbulence intensity) for motion initiation [3, 4]. Preliminary results from controlled flume experiments demonstrate threshold shifts across configurations, underscoring the sensitivity of bed stability to local topography. 
These insights aim to highlight the transformative potential of IMU-based instrumentation for real-time risk assessment of riverbed and bank destabilization in natural streams, as well as scour development in engineered channels, for sustainable river management and infrastructure resilience.
 
References
1. Al-Obaidi K, Xu Y, Valyrakis M. The design and calibration of instrumented particles for assessing water infrastructure hazards. J Sens Actuator Netw. 2020;9(3):36. doi:10.3390/jsan9030036.
2. Al-Obaidi K, Valyrakis M. A sensory instrumented particle for environmental monitoring applications: development and calibration. IEEE Sens J. 2021;21(8):10153-10166. doi:10.1109/JSEN.2021.3053080.
3. Al-Obaidi K, Valyrakis M. Linking the explicit probability of entrainment of instrumented particles to flow hydrodynamics. Earth Surf Process Landf. 2021;46(12):2448-2465. doi:10.1002/esp.5178.
4. Al-Obaidi K, Valyrakis M. Coherent flow structures linked to the impulse criterion for incipient motion of coarse sediment. Appl Sci (Basel). 2023;13(19):10656. doi:10.3390/app131910656.

How to cite: Papadaki, A. and Valyrakis, M.:  Influence of Pocket Geometry on the Incipient Entrainment of Coarse Particles in Turbulent Flows , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11632, https://doi.org/10.5194/egusphere-egu26-11632, 2026.

EGU26-12336 | Posters on site | GM2.6

Basal force distribution from steady fully-developed granular flows 

Hui Tang, Jun Fang, Yifei Cui, Jens Turowski, Lu Jing, and Yong Kong

Understanding the impact of geophysical flows on the channel bed is essential for assessing erosion processes of bed material. In this study, the discrete element method (DEM) is used to simulate idealized, steady-state, fully-developed granular flows impacting the channel bed with systematically varying total particle number (1000-30000), grain size (2-16mm), and slope angle (28-34°) to investigate the probability distributions of the basal force. The probability density functions of the basal force, normalized to the mean force, were calculated and fitted with ten probability distributions. Four indices, namely R2, Residual Sum of Squares (RSS), Wasserstein distance, and information entropy, are introduced to evaluate the goodness of fit for each probability density distribution. By comparison, the broad probability density distribution of normalized basal force can be well-described by Gamma distributions (GD) with its shape and scale parameters. The shape parameter of the Gamma distribution is positively correlated with the total particle number and grain size, but negatively correlated with the slope angle. An opposite relationship is revealed in the scale parameter of the Gamma distribution. Additionally, we analyzed flow kinematics by calculating the coordination number, dimensionless velocity, shear rate, inertial number, and volume fraction, and linking these variables to the shape and scale parameters. The coordination number, shear rate, inertial number, and volume fraction serve as effective proxies for the shape and scale parameters, enabling interpretation of the statistical characteristics of monitored basal forces in geophysical mass flows.

How to cite: Tang, H., Fang, J., Cui, Y., Turowski, J., Jing, L., and Kong, Y.: Basal force distribution from steady fully-developed granular flows, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12336, https://doi.org/10.5194/egusphere-egu26-12336, 2026.

EGU26-12572 | Posters on site | GM2.6

Multi-Modal Monitoring and Modelling of Extreme Hydro-Geomorphological Events: Bridging the Gap Between Local Dynamics and Catchment-Scale Predictions 

Anette Eltner, Michael Dietze, Julia Kowalski, Jochen Aberle, Jens Grundmann, and Bernhard Vowinckel

The central challenge in understanding extreme hydro-geomorphologic events is the persistent lack of integrated, quantitative observations capable of developing and constraining predictive models. While flash floods and associated sediment transport represent an escalating hazard under climate change, their underlying dynamics remain poorly understood across the spatio-temporal scales required for effective risk mitigation. Existing monitoring is often fragmented, with upcoming novel approaches only partly resolving key unknowns when used in isolation. For instance, optical methods such as UAV-based photogrammetry and camera gauges provide high resolution surface process data but cannot resolve subsurface bedload dynamics, whereas environmental seismic methods capture particle-riverbed interactions and signatures of turbulence but produce indirect, composite signals that are difficult to isolate and quantify.

To bridge this gap, we envision a multi-modal approach that moves beyond those single-technique or single-sensor proxies. To reliably and robustly observe temporarily evolving interlinked key parameters, i.e., water level, flow velocity, and hydraulic geometry, major steps involve using stereo-vision for precise scaling and channel cross-section updates, alongside AI-based optical flow for complex velocity fields. By integrating low-cost, event-triggered sensors (e.g., thermal & multispectral cameras, seismometers, and LiDAR), we can automate the retrieval of discharge as well as additional parameters such as turbidity and granulometry. Using photogrammetric change detection and AI-driven image processing we can further bridge terrestrial and aerial perspectives (e.g., from UAV), moving toward a physically consistent characterization of extreme events. By integrating high-resolution 3D imaging and seismic data inversion, it becomes possible to capture water and sediment dynamics simultaneously, resulting in unique complementary information on the same event.

In this framework, laboratory experiments provide the necessary controlled conditions to infer the capabilities, caveats and calibration measures for this sensor integration. Highly resolved computational fluid dynamics multiphase flow modelling will generate synthetic reference datasets to disentangle environmental signals and sensor noise. These heterogeneous data streams are integrated via AI-based fusion and uncertainty modelling to resolve non-linear relationships governing coupled water–sediment dynamics. Ultimately, hydrological and hydraulic modelling serves as a testbed for upscaling, in which models are informed by improved process knowledge-based observation data and its uncertainty to evaluate how small-scale insights alter catchment-scale predictions.

From this framework, significant gaps emerge that define the current research frontier. A critical unresolved challenge is the systematic separation of source terms from the superimposed signals generated by the actively evolving sediment-carrying river during flood events. Furthermore, the transition from "data-rich" local observations to “data-poor” but "process-informed" regional models is still hindered by the lack of scalable frameworks that can maintain physical consistency across different scales, i.e., climatic and geomorphological regimes. Addressing these gaps requires a coordinated shift from observing isolated parameters to an integrative, physics-based monitoring loop that can provide truly scalable, model-ready information for extreme events.

How to cite: Eltner, A., Dietze, M., Kowalski, J., Aberle, J., Grundmann, J., and Vowinckel, B.: Multi-Modal Monitoring and Modelling of Extreme Hydro-Geomorphological Events: Bridging the Gap Between Local Dynamics and Catchment-Scale Predictions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12572, https://doi.org/10.5194/egusphere-egu26-12572, 2026.

EGU26-12701 | Orals | GM2.6

Rheology of sedimentary flows across the viscous–inertial transition 

Bernhard Vowinckel, Alireza Khodabakhshi, Sudarshan Konidena, and Franco Tapia

Dense sedimentary flows underpin a wide range of geomorphic processes, from bedload transport in rivers to debris-laden shallow flows, yet their rheological description across regimes remains incomplete. In particular, the transition from viscous-dominated to inertia-dominated behavior in dense suspensions poses a central challenge for constitutive modeling of subaqueous sediment transport. Here, we present a unified numerical investigation of the viscous–inertial transition in sheared sedimentary flows using particle-resolved Direct Numerical Simulations (pr-DNS), spanning idealized rheometric configurations and flow-driven sediment beds.

We employ both pressure-imposed and volume-imposed rheological frameworks to systematically probe the role of fluid viscosity, shear rate, granular pressure, particle friction, confinement, and boundary roughness. Across configurations, we characterize rheology in terms of the macroscopic friction and solid volume fraction expressed as functions of combined viscous and inertial control parameters. Our results confirm that the transition can be described by an additive scaling of visco-inertial stresses but reveal that different rheological quantities respond differently to inertia.

In pressure-imposed simulations of dense frictional suspensions, we find that the viscous–inertial transition occurs at Stokes numbers ranging from 5 to around 8, consistent with recent experiments. Notably, shear stress exhibits a more gradual transition than particle pressure, indicating a decoupling of stress components. Microstructural analysis shows that this behavior arises from the combined action of lubrication and tangential contact forces, as particles progressively shift from rolling to sliding contacts. This shift is governed not only by the Stokes number, but also by proximity to jamming and inter-particle friction.

Complementary volume-imposed simulations between rough confining walls demonstrate that boundary conditions strongly influence the measured rheology through particle layering and inter-layer mixing. Wall roughness and cell height modulate stress levels and effective friction, including weakening of the macroscopic friction during the transition, while preserving a consistent viscous–inertial scaling across cases. Despite a reduction in contact number, increased force magnitudes on remaining contacts drive the inertial regime.

Finally, simulations of pressure-driven shallow flows over sediment beds show that the transition occurs at Stokes numbers comparable to those of our numerical and experimental results of pressure-imposed rheometry, with distinct scaling coefficients for volume fraction and macroscopic friction. Together, these results highlight the complex, multi-scale nature of sediment rheology and underscore the need for refined constitutive laws that explicitly account for microstructure, confinement, and stress anisotropy in geomorphic sediment transport.

How to cite: Vowinckel, B., Khodabakhshi, A., Konidena, S., and Tapia, F.: Rheology of sedimentary flows across the viscous–inertial transition, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12701, https://doi.org/10.5194/egusphere-egu26-12701, 2026.

EGU26-13379 | ECS | Orals | GM2.6

Resolved DNS of bedload transport with realistic grain morphology 

Ricardo Rebel and Jochen Fröhlich

The prediction of bedload sediment transport remains challenging due to the multi-scale interactions that link grain-scale dynamics, bed morphology, and turbulence. Grain-scale processes are influenced by particle shape and contribute to the spread in existing bedload models. Experimental access to these processes is limited, making numerical simulations a valuable complementary tool. Most numerical studies to date represent sediment grains as spheres to reduce computational cost or intentionally exclude shape effects. More recent work has demonstrated the importance of shape using ellipsoidal approximations which capture the overall grain form but loose finer surface irregularities. Only a few simulations have employed more realistic clumped-sphere grain approximations and have shown that grain shape introduces significant uncertainty in entrainment and transport predictions.

This contribution advances the quantification of grain-shape effects by using realistic representations of grain geometry obtained from measurements in the literature. It presents direct numerical simulations of turbulent bedload transport with low particle loading in a highly mobile regime using fully resolved, realistic sand grains. Three simulations with monodisperse but polymorph particles are considered, such that only grain shape is varied. One configuration represents smooth, well-rounded sand grains, the second consists of more angular and irregular grains. A third simulation with uniform spheres serves as a reference. The realistic grain samples are generated statistically following an established methodology that yields two distinct sand populations. The grains in these populations are characterized using sphericity and roundness and are classified using the Zingg diagram. Although the Zingg-class of all grains is spheroid, the grain populations can be subdivided based on the distributions of the other two shape descriptors, with sphericity capturing larger-scale morphology and roundness reflecting smaller-scale surface irregularities.

Across the three simulations, the Shields parameter increases with increasing grain irregularity. Furthermore, the particle ensembles in all simulations show oscillatory dynamics during statistically steady bedload transport, attributed to the recurring formation of particle clusters, with the characteristic period increasing with grain irregularity. Shape-conditioned statistics obtained through double averaging show that in the case of the angular grain population more rounded grains accumulate near the channel bottom, while more angular grains are transported to higher elevations. This sorting is not observed for the well-rounded grain population. Additionally, for both grain populations, the rotational energy of the grains increases with irregularity, although rotation remains overall weak compared to translational motion in the present highly mobile regime.

How to cite: Rebel, R. and Fröhlich, J.: Resolved DNS of bedload transport with realistic grain morphology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13379, https://doi.org/10.5194/egusphere-egu26-13379, 2026.

EGU26-15476 | Posters on site | GM2.6

The Edge of Stability: From Collective Vibrations to Jamming and Failure in Granular Media 

Pj Zrelak, Eric Breard, Symeon Makris, and Josef Dufek

Granular media is observed in a variety of natural contexts. Whether they come in the form of landslides, debris flows, pyroclastic density currents, bed load, fault gouge, or magmatic crystals, they can fail catastrophically and jam. Here we introduce a characterisation that examines collective motion within granular systems to probe their stability as they are pushed towards the point of failure and stoppage. Using particle-resolved simulations, we show that this characterisation gives early indication of weakening prior to external measures. This characterisation is agnostic to the method of destabilisation, whether it be from increasing slope angles or fluid injection. Applying this characterisation to analogue experiments shows that it can easily demarcate between a static deposit, agitated particles, and an actively destabilizing layer, showing promise in using remote signals to probe the stability of natural systems.

How to cite: Zrelak, P., Breard, E., Makris, S., and Dufek, J.: The Edge of Stability: From Collective Vibrations to Jamming and Failure in Granular Media, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15476, https://doi.org/10.5194/egusphere-egu26-15476, 2026.

Braided rivers are dynamic systems that support diverse habitats associated with their shifting mosaic of anabranches, backwaters, bars and islands. These units are characterized by chaotic, but not random, distributions of substrate, elevation and hydraulics at multiple scales. Modelling sediment supply or flow-driven changes in riverbed composition is notoriously difficult given the inherent dynamism and multiple scales defining large braided rivers.

In this research, we present a new data-rich modelling framework which combines census-scale [1 m] substrate classification with detailed 2D hydraulic models. The resulting transport capacity estimates can, for a static bed, be quickly applied to any transient flow scenario while retaining spatial detail. We then use the information gathered during the 2D modelling to parameterise a 1.5-dimensional transport solution in the time-evolving CASCADE sediment routing framework.

The 2D model uses a substrate map of a 56-km reach of the Rangitata [Rakitata] River, Aotearoa New Zealand, derived by machine learning based on high-fidelity helicopter lidar and orthophotography. A library of 2D steady-state hydraulic models is then run over the substrate map to predict the spatial and temporal capacity for sediment transport.

The adapted 1.5D-CASCADE model captures a defining feature of braided rivers, width variability, with a reach-specific hypsometric solver, tested against the 2D results, that predicts flow and sediment transport. The half-dimension is width, discretised against height using the 2D predictions of inundation and active area. The 1.5D model can then evolve bed composition both laterally across the braidplain and longitudinally down the river, within hydraulic geometry set by the template survey, including storage and remobilisation in side channels and floodplains.

The models are tested and applied to simulate the effects of flow regulation on bed composition in the Rangitata River. The model’s longitudinal consistency was only possible when using the spatial substrate data, and predictions are corroborated by lidar change detection. Results demonstrate that subtle changes in flow regime can alter where sediment is stored across the braidplain, with sedimentation impacts focused on side channels. Transfer of the model to other rivers indicates that width-varying solvers produce more stable sediment routing predictions than any single width, while remaining computationally efficient. 

How to cite: Rogers, J. and Brasington, J.: Adapting CASCADE for braided rivers: A 1.5D sediment transport approach with variable substrate and width, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15789, https://doi.org/10.5194/egusphere-egu26-15789, 2026.

EGU26-16255 | ECS | Posters on site | GM2.6

Shape Matters: How particle morphology affects the location ofthe Gravel-Sand Transition. 

Swagat Kumar Panda, Samantak Kundu, Sanjay Kumar Mandal, and Dirk Scherler

In foreland basins adjacent to collisional mountain belts, rivers exhibit an abrupt gravel-sand transition (GST) at ~10-40 km downstream of mountain fronts, where surface median grain size reduces from ~10 mm to ~1 mm. This is the only abrupt downstream reduction in grain size in fluvial systems. Existing theories attribute GST formation to size-selective transport of bimodal sediment, rapid deposition of sand from the washload, and gravel exhaustion. These mechanisms predict that GST location should respond systematically to changes in hydraulic conditions (channel gradient, flow strength), sediment supply (gravel flux), and accommodation space (subsidence rate). However, observations from the Himalayan foreland basin reveal significant along-strike variability in GST locations despite similar gravel lithology, comparable subsidence rates, and uniform climatic forcing. This unexplained spatial variability indicates that additional controls on GST formation remain poorly understood.

Here, we hypothesize that particle shape—an intrinsic sediment property traditionally considered secondary to grain size—exerts first-order control on GST location through its influence on gravel mobility. To test this hypothesis, we developed a force-balance framework accounting for drag, lift, and rotational forces to model gravel transport as a function of particle shape. Experiments with varying bed matrix characteristics demonstrate that gravel mobility is strongly modulated by shape variations under identical hydraulic conditions. Field measurements of particle shape distributions from Himalayan foreland rivers reveal that GST locations coincide spatially with downstream increases in the proportion of low-mobility shapes (equant and platy forms). Progressive accumulation of these less mobile shapes reduces the bulk mobility of the gravel bedload, causing the gravel front to stall.

Our results demonstrate that particle shape exerts first-order control on GST formation and location, operating independently of climate and tectonic forcing. This intrinsic control has likely influenced sediment routing in both ancient and modern foreland basins worldwide. The findings suggest that GST positions in stratigraphic records reflect the evolution of particle shape rather than solely changes in external forcing. Understanding this shape-controlled mechanism is essential for interpreting sedimentary archives, predicting downstream sediment delivery, and refining landscape evolution models in mountain-foreland systems.

How to cite: Panda, S. K., Kundu, S., Mandal, S. K., and Scherler, D.: Shape Matters: How particle morphology affects the location ofthe Gravel-Sand Transition., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16255, https://doi.org/10.5194/egusphere-egu26-16255, 2026.

EGU26-16411 | Orals | GM2.6

Bed shear stress in bedload transport: new methods of sidewall correction and bed surface determination 

Thomas Pähtz, Yulan Chen, Han Yu, Maoxing Wei, and Orencio Duran

The study-to-study variability of bedload flux measurements in turbulent sediment transport borders an order of magnitude, even for idealized laboratory conditions. This uncertainty stems from physically poorly supported, empirical methods to account for channel geometry effects in the determination of the transport-driving bed shear stress and from study-to-study grain shape variations. Here, we derive a universal procedure of bed shear stress determination. It consists of a physically-based definition of the bed surface and a channel sidewall correction that does largely not rely on empirical elements, except for well-established scaling coefficients associated with Kolmogorov's theory of turbulence. Application of this procedure to bedload transport of spherical grains---to rule out grain shape effects---collapses data from existing laboratory measurements and grain-resolved CFD-DEM simulations for various channel geometries onto a single curve. By contrast, classical sidewall corrections, such as the Einstein-Johnson method, as well as an alternative bed surface definition, are unable to universally capture these data, especially those from shallow or very narrow channel flows. The sidewall correction method is also independently supported by data from systematic experiments of open-channel flows over fixed rough beds with various width-to-depth ratios.

How to cite: Pähtz, T., Chen, Y., Yu, H., Wei, M., and Duran, O.: Bed shear stress in bedload transport: new methods of sidewall correction and bed surface determination, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16411, https://doi.org/10.5194/egusphere-egu26-16411, 2026.

EGU26-16480 | Orals | GM2.6

Vertical Velocity Profiles in Erosive Landslides 

Ivo Baselt, Michael Krautblatter, Shiva Pudasaini, and Katharina Wetterauer

Vertical velocity profiles in erosive multiphase mass flows control how momentum is transferred from a moving landslide to the underlying bed and therefore govern erosion, entrainment, and mass enhancement. Although erosion is known to increase landslide mobility, the particle-scale mechanisms by which internal shear drives sediment mobilisation remain poorly constrained. In particular, the vertical distribution of velocity in erosive granular flows is largely unknown, despite providing the critical link between flow dynamics and bed response. Field measurements document a wide range of velocity profile shapes but lack the spatial resolution required to quantify shear close to the bed. By contrast, previous laboratory studies either failed to resolve internal kinematics under erosive conditions or relied on artificial, rounded particles that suppress the frictional interactions characteristic of natural sediments. Consequently, differences between landslide velocity and the velocity of the eroded bed, as well as the vertical shear rates underpinning erosion-entrainment-mobility formulations, remain largely unconstrained by empirical data.

Here we present a new experimental dataset that directly addresses this gap. We conducted controlled laboratory experiments on landslide-like granular flows moving over an erodible bed composed of naturally crushed sand-gravel mixtures. A measurement approach based on Particle Image Velocimetry combines lateral imaging with plan-view observations, allowing continuous vertical velocity profiles to be reconstructed across the full flow depth during active erosion and entrainment. The experiments include dry granular flows and flows with varying water content, two representative grain-size classes, and systematic comparisons between erosive runs and reference cases over a rigid bed.

The results show that both the inertia of the erodible material and the time-dependent erosion rate fundamentally alter the vertical velocity profile. The velocity of the moving landslide and that of the erodible bed can now be clearly distinguished, enabling direct calculation of entrainment velocity and erosion drift. Shear mainly occurs near the bed-flow interface, evolving dynamically as material is entrained and creating velocity gradients that cannot be captured by depth-averaged approximations. These measurements provide the first quantitative characterisation of vertical shear under fully erosive conditions using realistic sediment properties. By resolving particle-scale velocity gradients, this study establishes the experimental basis required to calibrate and verify erosion-mobility models that explicitly depend on shear-rate-controlled entrainment, thereby advancing the predictive modelling of erosive landslides.

How to cite: Baselt, I., Krautblatter, M., Pudasaini, S., and Wetterauer, K.: Vertical Velocity Profiles in Erosive Landslides, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16480, https://doi.org/10.5194/egusphere-egu26-16480, 2026.

EGU26-16521 | ECS | Orals | GM2.6

Geomorphic and sedimentary records for deciphering the landform evolution at the Damodar and Barakar River confluence 

Surajit Kundu, Subhajit Sinha, and Sk Mafizul Haque

Fluvial dynamics hinge on sediment erosion, transport, and deposition. These are the forcing factors responsible for changing channel morphology and landform evolution. Our study analyses these processes at the confluence of the Damodar River and the Barakar River in eastern India. It is a transitional zone between Archaean-Proterozoic crystalline rocks, lower Gondwana formations, and Quaternary alluvium. The landscape remains in a constant state of change, shaped by the annual pulse of flood and profoundly altered by two hundred years of anthropogenic activity.

An integrated framework evaluates boundary conditions, morphologic responses, fluvial drivers, and terrace archives. Despite comparable flow velocities in active channels, rivers transport distinct grain sizes and lithologies. The right-bank remnants of the Damodar River evidence past high-energy regimes and are absent on the left bank. Terrace sequences are unpaired, sedimentologic units are unmatched, and bank structures preserve ancient high-velocity signatures.

How to cite: Kundu, S., Sinha, S., and Haque, S. M.: Geomorphic and sedimentary records for deciphering the landform evolution at the Damodar and Barakar River confluence, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16521, https://doi.org/10.5194/egusphere-egu26-16521, 2026.

Coupled interactions between climate, vegetation, and geomorphic processes control sediment export from rapidly eroding badlands; however, their relative roles under future climate scenarios remain poorly constrained. We present a coupled landscape evolution model (LEM) and a dynamic vegetation model, CLIMBAD, applied to the Laval catchment (Draix-Bléone CZO, SE France) in a badland setting, to quantify how fluvial and hillslope erosion, together with frost weathering and vegetation dynamics, drive historical and projected sediment fluxes. The LEM is forced by temperatures (acting on frost weathering) and precipitation events, including depth, duration, and peak intensity. The dynamic vegetation model is calibrated to 1982-2021 vegetation maps and driven by topographic and climatic variables. Future climate (2022-2099) is generated using a stochastic weather generator calibrated on observations from historical data and future projections obtained from a regional climate model.

Model evaluation for 1985-2021 shows that coupling dynamic vegetation to the LEM improves agreement with observed annual sediment fluxes at the catchment outlet (i.e., R2 increased from ~0.60 to ~0.66), demonstrating the importance of vegetation-erosion feedbacks. To isolate climatic controls, we ran four scenarios for future climate: (i) changing temperature (T) and precipitation (P), (ii) constant T with changing P, (iii) changing T with constant P, and (iv) constant T and P. These results help disentangle the relative contribution of a change in the precipitation regime and a change in temperature on sediment fluxes in a coupled system, with direct implications for sediment hazard assessment in climate‑sensitive badland landscapes.

How to cite: Sharma, H., Le Bouteiller, C., and Boulangeat, I.: Coupling Landscape Evolution and Dynamic Vegetation Models to Simulate Sediment Fluxes under Historical and Future Climate in the Laval Catchment (Draix-Bleone CZO, SE France), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19059, https://doi.org/10.5194/egusphere-egu26-19059, 2026.

EGU26-19202 | ECS | Posters on site | GM2.6

Surrogate-based sensitivity analysis and calibration for the hydro-sedimentary modeling of an elementary agricultural catchment 

marylin rubi uchasara huarachi, veronique gervais, John armitage, Christine franke, and claire alary

Landscape evolution models typically solve three main processes: the conversion of rainfall to runoff, flow routing, erosion, and sediment transport, for a given precipitation time series, and a topographic surface. They can help to predict watershed dynamics in response to potential extreme events and anticipate potential damages. To that purpose, models must accurately represent the studied catchment and reproduce available observations, such as water discharge and sediment flux. This requires adjusting the model parameters representing the catchment characteristics, which can be challenging due to long simulation times, many uncertain characteristics and modeling errors.  

This study focuses on modeling the Pommeroye catchment — a 0.54 km² elementary watershed in the Canche River basin in northern France. The objective is to identify models able to reproduce the twenty extreme events identified in the data collected during the 2016-2017 hydrological year for discharge and suspended sediment at the catchment outlet. Topography is derived from a high-resolution (1m) LiDAR-derived digital elevation model. CAESAR-Lisflood is considered for dynamic simulation. The rainfall-to-runoff is modeled with a local storage term that has an exponential recession and is controlled by the water storage depth parameter “m”. From the generated surface runoff, the model continuously computes the flux of water and sediment across cells. Flow routing is solved via a reduced solution to the shallow water equations, where the friction term is computed via the Manning-Strickler model and hence controlled by the Manning’s roughness. Sediment transport follows the Wilcock and Crowe parameterization, with multiple controlling parameters. For the Pommeroye catchment, model run times are long, e.g. up to 24 hours on 36 CPUs, limiting the number of simulations that can be performed in practice. To overcome this, we developed a workflow combining machine learning-based surrogate models with sensitivity analysis and calibration. Gaussian processes are considered to mimic CAESAR-Lisflood from a limited training set and provide fast estimations of the simulator outputs for any input parameter values within given ranges. Instead of CAESAR-Lisflood, these predictions are used for variance-based sensitivity analysis (Sobol’ indices) and optimization (Efficient Global Optimization), drastically reducing the computation times.

A first sensitivity analysis highlighted that the m parameter mainly affects water discharge. However, no single m parameter value enables the model to correctly reproduce all data: the best fit is obtained with increasing values throughout the year, starting with low values in winter. In a second study, we thus added flexibility with time-dependent monthly values for m, leading to an improved match with water discharge data. Finally, the EGO approach - with fixed monthly m values - was considered to better reproduce suspended sediment data, identifying settling velocity and Manning’s roughness as key factors.

How to cite: uchasara huarachi, M. R., gervais, V., armitage, J., franke, C., and alary, C.: Surrogate-based sensitivity analysis and calibration for the hydro-sedimentary modeling of an elementary agricultural catchment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19202, https://doi.org/10.5194/egusphere-egu26-19202, 2026.

EGU26-21488 | Orals | GM2.6

Evaluation of convection-permitting models for rainfall erosivity in an Alpine region 

Marco Borga, Ahmed Mansoor, Eleonora Dallan, and Marra Francesco

Rainfall erosivity is a major driver of soil erosion and is highly sensitive to short-duration precipitation extremes, which are expected to intensify under climate change. Great advancement on climate data have been seen in the last decade, and convection-permitting climate models (CPMs) offer new opportunities to simulate rainfall characteristics relevant to erosivity. However, their performance in complex terrain remains insufficiently quantified.

We evaluate rainfall erosivity (RUSLE R-factor) simulated by a nine-member CPM ensemble from the CORDEX Flagship Pilot Study on Convective Phenomena over Europe, focusing on the Great Alpine Region. CPM estimates are compared with long-term, high-resolution rain-gauge observations from ~500 stations spanning a wide elevation range. We quantify and apply a temporal adjustment to reconcile hourly model output with 10-minute observations, then model performance vs observations is assessed for key erosivity-related variables, including rainfall intensity, event depth, frequency of erosive events, and mean annual erosivity. The CPM ensemble reproduces the spatial variability of rainfall erosivity with good skill and overall low bias, but exhibits clear elevation-dependent biases. Erosivity is underestimated at low elevations and increasingly overestimated at higher elevations, reflecting biases in rainfall intensity and/or event frequency. While low-elevation biases are largely consistent with sampling variability, high-elevation biases are predominantly systematic.

These results highlight the potential of CPMs for rainfall erosivity assessment and the importance of accounting for elevation-dependent biases in mountainous regions.

How to cite: Borga, M., Mansoor, A., Dallan, E., and Francesco, M.: Evaluation of convection-permitting models for rainfall erosivity in an Alpine region, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21488, https://doi.org/10.5194/egusphere-egu26-21488, 2026.

EGU26-22114 | Posters on site | GM2.6

A model for the fluvial transport of different size and density classes 

Ana M Ricardo, Rui M L Ferreira, Arianna Varrani, Massimo Guerrero, Pawel Rowinski, and Magdalena Mrokowska

A numerical model is developed for the transport of mixed natural sediment and plastic particles, accounting for multiple size classes and material densities. The conceptual model drawn from a classico Hirano layered description. It includes a transport layer, an active layer and a substratum. In the transport layer mass conservation consists on fraction-wise Exner equations, including pickup and deposition rates, convective and diffusive transport in the transport layer, and local accumulation for each size and density class. Convective fluxes are the product of particle activity for each size and density classes (the conservative variables) and particle bulk velocity. The latter computed using a modified Luque and van Beek formulation, adapted to account for different sizes and particle densities. Thresholds for incipient motion are taken as calibration coefficients. A flux limiter is implemented to avoid over-saturation of the transport layer and to ensure positivity of particle activity. The pickup function is derived from probabilistic descriptions of sediment entrainment (taking into account density) and deposition rates are functions of actual particle activity and sedimentation velocity. The dynamics of the active layer is determined by empirical availability functions by size. The volume of the active layer is kept constant and scaling with the initial d90 of the mixture. Instantaneous mixing is assumed. As a consequence, during deposition the composition of the active is transferred to the substratum. During erosion, the composition of the substratum is incorporated in the active layer.

The model is calibrated with laboratory experiments conducted under steady and overfeeding flow conditions. Two flumes were employed. A 5.2 m long, 25 cm wide, and 35 cm deep flume was used to conduct flat-bed experiments in two scenarios: (i) homogeneous bed composed of plastic granules, and (ii) gravel or sand bed mixed with plastic granules, which were manually seeded at clastic bed surface for different covering percentage. A 12 m long, 40 cm wide channel was used to conduct gravel-sand sediment sorting experiments, leading to surface coarsening, and overfeeding experiments. Calibration consisted in finding best fits to threshold values of grain velocities, ensuring the observed equal mobility characteristics of poorly sediments with the same density. After calibration, the simulations reproduce the observed grave-sand sheet propagation in the overfeeding experiments. Simulations of the tests of different density classes indicate that coarse, low-density particles exhibit higher mobility than equally sized quartz particles, while the mobility of fine, low-density particles is comparable to that of natural sand of similar size. The model provides a consistent and conservative framework for representing the coupled transport and sorting of sediment–plastic mixtures in open-channel flows.

 

Acknowledgement: This works was supported by the Portuguese Foundation for Science and Technology (FCT) through project Project DT4Rivers COMPETE2030‐FEDER‐00760800 and European Union through Interreg Atlantic 2021-2017 project TRAP – EAPA_0122/2024

How to cite: Ricardo, A. M., L Ferreira, R. M., Varrani, A., Guerrero, M., Rowinski, P., and Mrokowska, M.: A model for the fluvial transport of different size and density classes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22114, https://doi.org/10.5194/egusphere-egu26-22114, 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.

EGU26-1349 | Posters on site | SSS6.1

Modeling Saline Soil Remediation Using the Surface Evaporation Capacitor Approach. 

Uri Nachshon, Rotem Golan, and Roee Katzir

Soil salinization is a pervasive problem in arid environments, frequently exacerbated by anthropogenic activities. Remediation commonly involves soil leaching through natural precipitation or controlled, human-made flooding events. Accurate prediction of solute transport during these leaching processes is complex, as it is controlled by soil physical and hydraulic properties, climatic conditions, evaporation rates, and the volume and timing of infiltration. Precise physically-based numerical models are necessary for exact descriptions but demand detailed input regarding soil and environmental parameters.

This study examines a simplified, physically-based alternative: the Surface Evaporation Capacitor (SEC) concept proposed by Or and Lehmann in 2019. Originally developed to predict soil porewater evaporation, the SEC model posits that porewater shallower than the soil capillary length is consumed by surface evaporation, while deeper porewater remains protected from this process.

We adopt the SEC concept to estimate solute dynamics within the vadose zone and predict long-term salt accumulation profiles. By integrating soil capillary length, ambient evaporation, and the depth of natural or artificial wetting, the SEC allows for a simple determination of salt fate, specifically estimating the leaching depth required to prevent salinization in the root zone and near the surface.

We validated the SEC approach by comparing its predictions against detailed field measurements collected in a super-arid region of Israel, alongside results from a detailed physically-based numerical model. Results confirm the Evaporation Capacitor Model's validity as an accurate proxy for estimating annual solute dynamics and salt accumulation in saline soils. While the complex numerical model provides exact temporal descriptions, the simplified SEC model offers an accurate  and easily implementable net estimation of salt transport, making it highly valuable for large-scale practical remediation assessment and management.

How to cite: Nachshon, U., Golan, R., and Katzir, R.: Modeling Saline Soil Remediation Using the Surface Evaporation Capacitor Approach., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1349, https://doi.org/10.5194/egusphere-egu26-1349, 2026.

EGU26-2306 | ECS | Orals | SSS6.1

Size effects of desiccation cracking behavior in clayey soil 

Zhaolin Cai, Qing Cheng, Chao-Sheng Tang, Xin-Lun Ji, Jin-Jian Xu, Ying-Dong Gu, and Bin Shi

Desiccation cracking significantly impacts the engineering properties of soils, influencing fluid infiltration and structural stability. A key phenomenon in desiccation cracking is the size effect, where soil dimensions, including thickness and radius, alter cracking behavior. However, the size effect remains poorly understood, particularly in linking laboratory-scale findings to field conditions. Existing studies are often limited to small laboratory samples, leading to discrepancies in crack behavior across scales and a lack of standardized guidelines for determining suitable sample sizes in laboratory tests. This study investigates the size effect on desiccation cracking in clayey soils and identifies suitable laboratory sample sizes to represent field-scale cracking patterns. Desiccation tests were performed on soil samples with varying radii (25-100 mm) and thicknesses (5-18 mm). Cracking behavior during drying and equilibrium-state crack patterns were analyzed. A size parameter (λ), defined as the ratio of sample radius to thickness, was introduced to characterize the soil's volumetric size. Results reveal three distinct stages of the size effect: (i) the crack-free stage (λ <λc), with no visible cracks; (ii) the size-dependent stage (λc <λ <λt​), where cracking behavior changes significantly; and (iii) the size-insensitive stage (λ >λt​), where crack parameters stabilize. Two critical size parameters, the critical cracking size (λc ≈4.0) and the transition size (λt ≈9.0), were identified. The proposed size thresholds (λc and λt​) were found to be applicable across different clayey soils, suggesting the general relevance of the framework for scaling desiccation cracking behavior in diverse geotechnical contexts. These findings enhance the understanding of size effects and provide a framework for optimizing laboratory tests to better reflect field conditions.

How to cite: Cai, Z., Cheng, Q., Tang, C.-S., Ji, X.-L., Xu, J.-J., Gu, Y.-D., and Shi, B.: Size effects of desiccation cracking behavior in clayey soil, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2306, https://doi.org/10.5194/egusphere-egu26-2306, 2026.

EGU26-2422 | ECS | Posters on site | SSS6.1

Modeling reference water vapor adsorption in desert soils 

Mulugeta Weldegebriel Hagos, Dilia kool (RIP), and Nurit Agam

Non-rainfall water inputs (NWRIs; i.e., dew, fog, and water vapor adsorption (WVA)) are significant sources of water in arid environments. Amongst all NRWIs, WVA is likely the most common, yet it is the least studied. There is increasing evidence that water vapor adsorption occurs in many arid and hyper-arid regions, that together occupy 26% of the earth’s terrestrial surface. Quantifying WVA is therefore essential to fully understand the water cycle in these regions. While some studies quantified WVA as a function of the surface properties, they were either laboratory trials or limited to a specific location. No studies, to date, have presented a general model to quantify WVA. Given the complexity of the process, we propose an initial step towards bridging this knowledge gap, with the introduction of a new “reference water vapor adsorption” (Ao). Ao is the adsorption of water vapor from the atmosphere to a reference surface, conceptually similar to the “reference evapotranspiration” (ETo) that quantifies the evapotranspiration rate from a reference surface. We propose to calculate Ao as Ao = raCp(ea-es)/lgra where ρa is the density of air, Cp is the specific heat capacity of air, ea and es are the water vapor pressure in the air and in the air-filled pores, respectively, γ is the psychrometric constant, and ra is the aero dynamic resistance. Assuming a completely dry surface (similarly to assuming well-watered crop to calculate ETo), es is set to zero. To test this new concept, we conducted measurements in the Negev desert, Israel, from July to October 2025. Ao was calculated from continuous measurements of temperature and relative humidity at 2m height, and wind speed at two heights (3 and 0.8 m). In parallel, Ao was directly measured every two hours during multiple 24-h campaigns by exposing dry silica gel to the atmosphere. The calculated Ao followed closely the trend of measured Ao, encouraging further development of this index, and potentially allowing mapping of reference adsorption based on simple meteorological measurements.

How to cite: Hagos, M. W., kool (RIP), D., and Agam, N.: Modeling reference water vapor adsorption in desert soils, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2422, https://doi.org/10.5194/egusphere-egu26-2422, 2026.

EGU26-7438 | Orals | SSS6.1

The effect of soil macro-structure on bare soil evaporation 

Frederic Leuther, Mathilde Nielsen, and Efstathios Diamantopoulos

Evaporation of soil water is often characterised by water losses over time for a defined soil volume where soils are assumed to be homogeneous in texture and structure. In this study, we hypothesised that evaporation depends not only on climatic conditions, soil texture, and soil hydraulic properties but also on the soils’ macro-structure. Specifically, that the different distribution of air-filled macropores, stones, and the connectivity of soil matrix will affect bare soil evaporation and herewith the transition from stage 1 to stage 2 evaporation. In a climate constant room, we measured evaporation characteristics of undisturbed soil cores taken under various land uses and soil textures (clay and sandy loam) and compared the evaporation rates to columns with sieved soil repacked to the same bulk density. Tensiometers installed in two different depth provided information about the hydraulic gradient along the columns, while weight measurements continuously recorded the mass loss. Soil structure of undisturbed columns was determined by X-ray computed tomography (X-ray µCT) at a voxel size of 50 µm. In addition, we evaluated the effect of macro-structure on bare soil evaporation for unsaturated condition, i.e. visible porosity was air-filled, by 3D image-based simulations using HYDRUS 3D.  The lab study showed that the well-sorted repacked samples lost significantly more water as the undisturbed samples. The differences cannot be explained by the total porosity and thus the total water reservoir. When using the time, the hydraulic gradient along the undisturbed columns was exponentially increasing, it was shown that the well-connected macropore volume could explain most of the evaporation characteristics. In addition, the presence of denser soil clods significantly shortened the time to build up the gradient. Neither stone nor particulate organic matter content had a significant effect on evaporation characteristics. The 3D image-based simulation indicated that air-filled macropores act as barriers for upward water flow and that the loss of water was limited by the connectivity of the soil matrix. It can be concluded that not only soil texture effects bare soil evaporation but also the soil macro-structure.

How to cite: Leuther, F., Nielsen, M., and Diamantopoulos, E.: The effect of soil macro-structure on bare soil evaporation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7438, https://doi.org/10.5194/egusphere-egu26-7438, 2026.

EGU26-10739 | ECS | Posters on site | SSS6.1

Evaluation of the volume of influence of four tubular capacitive probes 

Amelia Bellosta-Diest, Miguel Echeverría, and Miguel Ángel Campo-Bescós

Efficient water management is a critical challenge in agriculture, particularly in regions such as Navarra, Spain, where irrigation accounts for up to 87% of total freshwater consumption. Capacitive soil moisture probes are widely adopted in precision agriculture; however, a notable inconsistency persists between the sensing ranges claimed by manufacturers (typically 5–15 cm) and those reported in the scientific literature (generally <6 cm). This discrepancy arises largely from the absence of standardized criteria to define the effective sensing volume of these sensors.

This study presents a replicable empirical methodology to characterize the volume of influence of four commercially available capacitive probes: AquaCheck, EnviroPro, Gerbil, and Sentek. Controlled laboratory experiments were conducted under air and water conditions, using 0.2 mm paper layers to incrementally simulate increasing distances from the moisture source. Sensor outputs were normalized to enable direct comparison across heterogeneous measurement units, including Volumetric Water Content (VWC%) and Scaled Frequency Units (SFU%).

All probes exhibited a logarithmic decrease in signal intensity with increasing distance from the water source. By modeling the sensing domain as a cylindrical volume with a 10 cm height and defining its effective extent at the 99.5th percentile of cumulative signal response, substantial differences among probes were observed. The estimated sensing volumes ranked as follows: Gerbil (710.59 cm³), EnviroPro, AquaCheck, and Sentek (236.71 cm³).

The results demonstrate that sensing volumes vary considerably among manufacturers and are strongly dependent on the percentile threshold used to define the effective volume of influence. These findings confirm the lack of uniformity in probe sensing behavior and underscore the need for technical standardization. Although derived from controlled laboratory conditions and therefore comparative in nature, the results provide critical insight for interpreting soil moisture measurements and offer a more reliable technical basis for informed decision-making in irrigation management.

How to cite: Bellosta-Diest, A., Echeverría, M., and Campo-Bescós, M. Á.: Evaluation of the volume of influence of four tubular capacitive probes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10739, https://doi.org/10.5194/egusphere-egu26-10739, 2026.

EGU26-13322 | Posters on site | SSS6.1

Scale Dependence of Soil Hydraulic Properties Obtained from Evaporation Experiments: Effect of Sample Height 

Prabhudutta Khatua, Jannis Bosse, Bhabani S. Das, Wolfgang Durner, and Sascha C. Iden

Climate-induced droughts and increasingly erratic precipitation patterns are stressing water resources and underscore the need for a better understanding of soil water flow and storage. Soil hydraulic properties, in particular the water retention curve and the hydraulic conductivity curve, are fundamental inputs for predicting soil water dynamics and for simulating variably-saturated flow with the Richards equation. The simplified evaporation method is a common laboratory technique for estimating SHP. It relies on linearization assumptions that introduce only negligible errors when sample heights are small. While a handful of theoretical studies have addressed how sample height affects SHP estimates, a systematic experimental assessment of this scale-dependence is still lacking.

We performed evaporation experiments on packed soil columns (5, 10 and 15 cm high) using both a sandy and a silty soil. Throughout each run, we recorded column mass to track water content and evaporation rate, and we measured matric potential with mini-tensiometers.  Applying the simplified evaporation method, we derived point data for the water retention curve and hydraulic conductivity curve. A flexible model which accounts for capillary and non-capillary storage and flow was fitted to the data using the program SHYPFIT. Inverse simulations with Hydrus-1D were then applied to assess the influence of sample height without relying on the assumptions of the simplified evaporation method. This allowed to discriminate between an actual scale-dependence of soil hydraulic properties and differences which are caused by the assumptions of the simplified evaporation method.

Our findings reveal that column height has a minimal impact on the water retention curve, with a tendency of a slight broadening of the pore size distribution and a modest increase in residual water content. The effect on hydraulic conductivity was even less pronounced. The results of inverse simulations substantially attenuate these height-related discrepancies in soil hydraulic properties, leaving only marginal differences.

How to cite: Khatua, P., Bosse, J., Das, B. S., Durner, W., and Iden, S. C.: Scale Dependence of Soil Hydraulic Properties Obtained from Evaporation Experiments: Effect of Sample Height, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13322, https://doi.org/10.5194/egusphere-egu26-13322, 2026.

EGU26-14166 | Orals | SSS6.1

Multifractal fingerprints of rain events on soil moisture and respiration in a Mediterranean grassland 

Ernesto Sanz, Victor Cicuendez, Rosa M. Inclán, Carlos Yagüe, and Ana M. Tarquis

Mediterranean grasslands operate near the edge of water limitation and are strongly driven by short, discrete rainfall events. Yet, we still know little about how the event-scale dynamics of soil moisture (SWC), soil temperature (ST) and soil respiration (reorganize between wet and dry years. Here we use multifractal detrended fluctuation analysis (MFDFA) on time series in El Escorial (central Spain) to characterise post-rain dynamics in two contrasting years: a relatively wet year (2022) and a dry year (2024). We focus on April (spring) and September (), and six series and interactions of the soil–plant–atmosphere system: SWC, ST, CO₂ and the pairs SWC–ST, SWC–CO₂, ST–CO₂. For each post-rain window (several days after individual events) we quantify for these six series, and compare their behaviour across seasons and years.

In April 2022, Δα is moderate and H2 shows a stable, moisture-dominated backbone: SWC–SWC and SWC–ST are highly persistent, while CO₂–CO₂ and ST–CO₂ are often antipersistent while still moderately multifractal, indicating that CO₂ acts mainly as a reactive signal to water and temperature. In April 2024, Δα increases markedly for CO₂–CO₂ and SWC–CO₂, and their H2 shifts towards stronger persistence, while ST–CO₂ becomes more antipersistent. This points to a reorganisation whereby, under early-season water stress, carbon–moisture couplings become the main carriers of complexity and memory, and ST becomes a more reactive pathway. In September 2022, multifractality remains moderate but a strongly negative asymmetry in SWC–SWC and SWC–CO₂ reveals sharp rewetting and respiration pulses driven by soil moisture. In September 2024, Δα becomes very high for SWC–SWC, SWC–ST and CO₂–CO₂, with H2 ≈ 0.9–1.0 for SWC–SWC, SWC–ST and CO₂–CO₂, while asymmetry shifts: extremes move from moisture-dominated (negative in SWC–CO₂) to carbon-dominated (positive in CO₂–CO₂) and ST–CO₂ becomes strongly antipersistent.

In conclusion, these results show that using SWC, ST and and their interactions it is possible to identify distinct post-rain “modes” of ecosystem functioning: (1) a wet-year regime with a persistent SWC–ST backbone and moisture-driven pulses, and (2) a dry-year regime where long-range memory strengthens in SWC–ST–CO₂ but extremes and intermittency shift into the carbon subsystem, indicating loss of hydrological buffering and increased carbon–thermal stress after rainfall events. Such event-scale indicators could be used to inform adaptive grassland and land management strategies in Mediterranean regions, by identifying when ecosystems are approaching critical thresholds of water and carbon stress.

Acknowledgement: This paper is part of the project Clasificación de Pastizales Mediante Métodos Supervisados—SANTO, from Universidad Politécnica de Madrid (project number: RP220220C024). And funded by the European Union. Views and opinions expressed are however those of the author(s) and do not necesarily reflect those of the European Union or European Research Executive Agency (REA). Neither the European Union nor the granting authority can be held responsible for them.

How to cite: Sanz, E., Cicuendez, V., Inclán, R. M., Yagüe, C., and Tarquis, A. M.: Multifractal fingerprints of rain events on soil moisture and respiration in a Mediterranean grassland, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14166, https://doi.org/10.5194/egusphere-egu26-14166, 2026.

EGU26-14368 | ECS | Orals | SSS6.1

Development of an in situ monitoring system for tracking solutes and gas emissions in soil 

Luciano Melo Silva, Simon Schwingenschuh, Minsu Kim, Jens Weber, Christian Holeček, Thomas Birngruber, Bettina Weber, and Stefanie Maier

Soil is a complex medium that supports numerous biological and chemical processes across multiple phases. The transformation of inorganic and organic compounds can lead to the accumulation of harmful substances in soil and the emission of reactive gases that affect air quality and climate. However, quantitative measurements remain limited by the lack of methods for in situ monitoring of multiphase processes and by approaches restricted to one or a few compounds at a time, measured either in the liquid or the gas phase. Thus, gaps persist in quantifying and monitoring transformation processes occurring at the gas-liquid interface.

Here, we describe a newly developed method to continuously measure gas fluxes and solute concentrations in soil by coupling a dynamic gas flux chamber (DC) with an open-flow microperfusion (OFM) technique, hereafter termed OFM-DC. The latter OFM method had previously been applied in medicinal research for drug development, and we have optimized it for the utilization in soil. OFM enables the continuous sampling and concentration measurement of soil solutes (e.g., microbial metabolites) in both laboratory and field settings, whereas DC quantifies soil trace-gas emissions (e.g., CO2, NOx, and HONO) over time.

We will present first experiments using the novel setup with synthetic soil systems that have characterized microbial activity and chemical properties. Our case studies on in situ measurements of microbial nitrogen (N) processes and reactive N gas (NO, HONO) emissions reveal the effectiveness of our methods for investigating multiphase soil transformation mechanisms under dynamic soil water conditions.

The OFM–DC measurement setup demonstrates its potential for long-term field monitoring of soil–air quality and the related impacts on planetary health. The obtained data can support improved soil management, which in turn can minimize soil degradation and trace-gas emissions.

How to cite: Melo Silva, L., Schwingenschuh, S., Kim, M., Weber, J., Holeček, C., Birngruber, T., Weber, B., and Maier, S.: Development of an in situ monitoring system for tracking solutes and gas emissions in soil, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14368, https://doi.org/10.5194/egusphere-egu26-14368, 2026.

EGU26-16325 | Posters on site | SSS6.1

Differences in soil water retention properties and plant available water below trees and grasses in a Mediterranean savanna 

Max Wittig, Sinikka J. Paulus, Gerardo Moreno, Arnaud Carrara, Laura Nadolski, Anke Hildebrandt, and Sung-Ching Lee

Feedback loops between plants and soil shape and stabilize plant communities. In savanna-like landscapes, which are common in arid and semi-arid regions, trees and grasses coexist at close spatial scales. These different growth forms can influence soil formation and properties within just a few meters of each other.

In this study, we investigate soil hydraulic properties in an extensively managed Holm oak savanna-like ecosystem (Dehesa) in central Spain by comparing soils beneath trees and in adjacent open grass areas. We analyze saturated hydraulic conductivity, soil water characteristic curves, derived parameters such as field capacity and permanent wilting point, and associated soil texture and organic carbon content. In addition, we analyze a 10-year time series of in situ soil water content and micrometeorological variables within microhabitats to determine whether differences in the static properties also translate into water availability differences within the ecosystem.

On average, the topsoil below trees contained 6.2% more pore space within the range of plant-available water than the topsoil below open grass areas. This was associated with, and likely driven by, higher levels of organic carbon beneath the trees. There was no significant difference in clay content between the two microhabitats. 

However, field observations of soil moisture showed high heterogeneity, with the soil beneath the trees not remaining significantly wetter than in the open area despite the higher storage capacity and reduced radiative energy input due to shading. Data from two eddy covariance towers showed that, unlike grasses, trees sustain transpiration throughout the year, suggesting enhanced water uptake near the trunk.

Together, these results illustrate how different vegetation types affect the same soil just a few metres apart. They also show that, although trees increase soil water storage capacity, it remains unclear whether this positive effect is offset by the large amounts of water extracted by trees and higher interception losses, ultimately leading to the soil being similarly dry beneath trees as in the open area during the Mediterranean summer.

How to cite: Wittig, M., Paulus, S. J., Moreno, G., Carrara, A., Nadolski, L., Hildebrandt, A., and Lee, S.-C.: Differences in soil water retention properties and plant available water below trees and grasses in a Mediterranean savanna, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16325, https://doi.org/10.5194/egusphere-egu26-16325, 2026.

EGU26-16443 | Orals | SSS6.1

The International Soil Moisture Network (ISMN): A data service providing free access to in situ observations 

Matthias Zink, Tunde Olarinoye, Fay Böhmer, Kasjen Kramer, and Wolgang Korres

Soil moisture is a key variable impacting land–atmosphere interactions, hydrological extremes, ecosystem processes, and agricultural productivity among others. Reliable in situ observations are essential for understanding soil moisture dynamics and for evaluating satellite-based products and land surface models. However, ground-based soil moisture measurements are often scattered across independent networks and remain difficult to access in a harmonized form. The International Soil Moisture Network (ISMN) was established to overcome these limitations by providing a global, freely-accessible repository of quality-controlled in situ soil moisture observations. Its mission is to support Earth system science, remote sensing validation, and model development through standardized and traceable soil moisture data.

The ISMN collects soil moisture time series from a wide range of regional, national, and international monitoring networks. Contributing datasets are harmonized in terms of format, metadata, and temporal resolution and undergo a consistent quality control procedure. The database includes multi-depth measurements across diverse climates, land cover types, and soil conditions, complemented by ancillary site information. Data are distributed through a dedicated web interface (https://ismn.earth), enabling efficient data discovery and use for large-scale and local studies.

Ongoing efforts are focusing on expanding the database by incorporating additional stations and data providers from institutional or governmental sources, as well as enhancing data quality and consistency to support more robust long-term analyses. Further resources are directed towards fortifying the operational system and improve usability to better serve our users. Beyond research applications, the ISMN increasingly contributes to the data-to-value chain of international initiatives that are led by the World Meteorological Organization (WMO), the Food and Agriculture Organization (FAO), and the Global Climate Observing System (GCOS). One example is the contribution of ISMN data to WMO’s annual State of the Global Water Resources report, supporting global assessments of hydrological conditions.

How to cite: Zink, M., Olarinoye, T., Böhmer, F., Kramer, K., and Korres, W.: The International Soil Moisture Network (ISMN): A data service providing free access to in situ observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16443, https://doi.org/10.5194/egusphere-egu26-16443, 2026.

Soil salinization dynamics are driven by complex interactions among climatic conditions, hydrological processes, and anthropogenic activities. Due to this complexity, traditional single global models often struggle to capture spatial heterogeneity, leading to high prediction uncertainty and limited robustness at the pixel scale.

To address these challenges, this study proposes a multi-source data-driven framework based on environmental similarity matching to enhance prediction adaptability in heterogeneous environments. We compiled a dataset of approximately 35,000 topsoil samples from arid and semi-arid regions and constructed a multidimensional covariate system grounded in soil-forming factor theory. The framework comprises three components: (1) heterogeneity-based stratification, partitioning samples by climate and land use; (2) model library construction, developing candidate machine learning ensembles within each stratum via repeated cross-validation; and (3) similarity-based prediction, which employs Gower distance to quantify environmental similarity between target locations and training samples to select the optimal model.

Evaluations indicate that the Random Forest algorithm exhibits robust stability across stratified regions. Compared to single models, the environment similarity–constrained selection strategy significantly improved performance in heterogeneous regions; notably, the coefficient of determination (R2) in arid cropland areas increased from 0.748 to 0.807. Feature contribution analysis supports the necessity of stratified modeling, revealing that soil salinity in arid regions is primarily driven by vegetation variables and geographic, whereas remote sensing indices and soil pH dominate in semi-humid regions. The methodological framework developed in this study provides a new approach for high-precision soil salinity mapping.

KEYWORDS: Soil salinization; Environmental similarity; Heterogeneous environments; Machine learning.

How to cite: She, X., Frankl, A., and Luo, G.: Soil salinization prediction for heterogeneous environments: an environmental similarity–based modeling framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16578, https://doi.org/10.5194/egusphere-egu26-16578, 2026.

Numerous reviews and meta-analyses have examined the vast body of literature evaluating the impact of the different agricultural soil preparation or of the various steps of cultural itinerary on plant growth, water regulation, carbon storage, etc… in short, on soil functions and services, which inherently depends on the soil processes occurring at the pore scale.

For example, the largest pores in the soil (macropores) significantly contribute in regulating the soil water cycle, as they improve infiltration capacity and drainage rates. There is however limited knowledge about the interactions between initial and boundary conditions with the topology and geometry of macropore networks in natural soils, and their influence on water flow. More long-term monitoring data, and dynamic experimentations, are needed to evaluate and model the impact of agricultural management practices on the soil resilience to maintain its functions.

One method to quantify the arrangement and the size distribution of the soil macropore network is X-ray computed tomography (X-ray CT), which is now routinely used world-wide. Images acquisition, pre- and post-processing, and pore structure quantification protocols are increasingly refined and tending towards standardization, thereby contributing to shared and comparable knowledge.

We initiated a research project aiming at monitoring the soil macropore network in agricultural soil and evaluate its response to different management practices (tillage recovery and multispecies cover cropping) using X-ray CT. We are developing a sampling device to extract soil samples (100 cm³) for analysis with X-ray µCT at time zero, after which the samples will be reinserted and embedded into the field for a six-months period before being extracted again. This process will be repeated at least four times.

We hypothesize that tillage, occurring above the sample, where it creates a connected isotropic soil pore structure with a low spatial extent, will modify the living and biochemical equilibrium of the soil and therefore modify the macropore network inside the sampling cylinder, located below the plough pan. On the opposite, we estimate that resistant macropore would remain when no tillage is applied, with an increased resistance under a covered soil. We also hypothesize that persistent macropore network is preferentially used by the main plant roots, as the macropores network created by roots is also the primary contributors of the network connectivity.

The experimental set up will be installed in the field in February 2026 for a short-term trial involving monthly sample extractions in order to assess the feasibility and accuracy of the method. The study per se will be conducted afterwards.  We will present the encountered challenges with this initial trial as well as the first quantifications of temporal changes of the soil macropore network with time.

Sarah Smet, as a post-doctoral research fellow, acknowledges the support of the National Fund for Scientific Research (Brussels, Belgium).

How to cite: Smet, S.: Challenges in monitoring the undisturbed top soil pore scale structure of an agricultural field, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17900, https://doi.org/10.5194/egusphere-egu26-17900, 2026.

EGU26-18251 | Posters on site | SSS6.1

Between two Furrows: Soil bulk density from Non-Invasive Seismology 

Maria Tsekhmistrenko, Joe Collins, Jeroen Ritsema, Simon Jeffery, and Tarje Nissen-Meyer

Soil is a critical resource for global food security, yet conventional physical soil analyses, remote sensing and geophysical methods are often labour-intensive and time-consuming. This study explores the potential of ultra-high-frequency (>500 Hz) hammer-source seismology to characterise soil physical properties at the decimetre scale.

Field experiments were conducted within a long-term trial near Harper Adams University (UK) comparing Conservation and Conventional agricultural practices. Two 1.5 m transects were surveyed in each treatment using 16 geophones, with soil samples collected at matching horizontal resolution. P-wave velocity (vp) was estimated in the upper 40 cm of the soil profile and compared with bulk density derived from physical samples.

Results show a strong and statistically significant correlation between vp and bulk density. This relationship is consistent throughout the depth profile, with good agreement between seismic velocity images and interpolated bulk-density measurements from soil cores. The findings demonstrate that ultra-high-frequency seismic methods can reliably resolve small-scale soil structure relevant to agricultural management.

Our results indicate that ultra-high-frequency seismic analysis is a promising and cost-effective approach for estimating soil bulk density. This technique has clear potential to support agronomic and land-management decision making.

How to cite: Tsekhmistrenko, M., Collins, J., Ritsema, J., Jeffery, S., and Nissen-Meyer, T.: Between two Furrows: Soil bulk density from Non-Invasive Seismology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18251, https://doi.org/10.5194/egusphere-egu26-18251, 2026.

EGU26-18983 | Posters on site | SSS6.1

Virtual Soil Simulator -  unsaturated pore media water transport model including film flow and isothermal vapor transport phenomena 

Krzysztof Lamorski, Maciej Kozyra, and Cezary Sławiński

Simulation of unsaturated water movement in porous media has conventionally been based on the Richards equation (RE), coupled with hydraulic conductivity functions that account solely for capillary-driven liquid flow. This approach, however, overlooks the presence of thin water films adsorbed on solid surfaces, which may contribute appreciably to transport processes under moderately dry to dry conditions. Recent advances, particularly the Peters–Durner–Iden (PDI) framework, enable a physically consistent representation of film flow and isothermal vapor diffusion within formulations of unsaturated hydraulic conductivity.

In this work, we introduce the Virtual Soil Simulator, a finite-volume, OpenFOAM-based implementation of the RE augmented with the PDI model to explicitly represent capillary, film, and vapor transport processes. Model performance was assessed using a suite of benchmark tests with analytical or well-established numerical reference solutions, including one-dimensional infiltration, infiltration under steep hydraulic gradients, and two-dimensional nonlinear infiltration scenarios. The results demonstrate high numerical accuracy and robust mass conservation.

The applicability of the model is further demonstrated through two case studies. In the first, inverse simulation of a 12-day soil core drying experiment showed that the classical RE formulation reproduced measurements only during the early, wet stage, whereas the PDI-enhanced model remained consistent with observations over the entire drying period and accurately represented regimes dominated by film and vapor flow. In the second case, a synthetic desaturation analysis conducted across 467 soil types indicated that film flow markedly accelerates drainage, with significant effects persisting even at comparatively high pressure heads (−10 m). These findings indicate that neglecting film flow leads to systematic underestimation of unsaturated hydraulic conductivity and distorted predictions of drying and drainage behavior. Moreover, simulations at very low pressure heads emphasize that reliable representation of transport processes requires the combined consideration of both film and vapor fluxes.

Acknowledgments

This research was founded by the National Science Centre within contract 2021/43/B/ST10/03143.

How to cite: Lamorski, K., Kozyra, M., and Sławiński, C.: Virtual Soil Simulator -  unsaturated pore media water transport model including film flow and isothermal vapor transport phenomena, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18983, https://doi.org/10.5194/egusphere-egu26-18983, 2026.

EGU26-19707 | Orals | SSS6.1

Contrasting perspectives on soil evaporation in soil science and land surface modelling 

Jan De Pue, José Miguel Barrios, William Moutier, and Françoise Gellens-Meulenberghs

Soil evaporation is an essential component of the hydrological cycle. Within soil science, the fundamental mechanisms involved in soil evaporation are well-documented. However, within the realm of land surface modelling, the coarse spatial and temporal scale, as well as the computational limitations result in a simplified representation of this highly non-linear process.
Here, we evaluated the current representation of soil evaporation within the RMI evapotranspiration (ET) and surface turbulent fluxes (STF) model applied in the frame of  the EUMETSAT Satellite Applications Facility  (LSA)  on support to Land Surface Analysis (SAF) (http://lsa-saf.eumetsat.int/). This model is used to produce remote-sensing based estimates of the fluxes, using Meteosat Second Generation (MSG) observations. With 30 minutes interval, estimates of these fluxes are provided in near real time, resulting in a data record that spans over 20 years.
We highlighted the discrepancies between the simplified representation of soil evaporation and the soil physical solution. To achieve this, synthetic experiments were performed using Hydrus as a reference for comparison with the LSA SAF ET-STF model. Additionally, a comparison was made with formulations in other land surface models (Surfex, ECLand & GLEAM), the resulting texture-dependent bias was demonstrated and impact of sub-grid heterogeneity was shown. Finally, an updated formulation was tested in large-scale ET simulations and evaluated using in situ observations.
Though widely recognised as one of the fundamental processes in the hydrological cycle, the perspective on soil evaporation is very different in soil physics compared to land surface modelling. Here, we attempted to harmonize both approaches in a pragmatic manner.

How to cite: De Pue, J., Barrios, J. M., Moutier, W., and Gellens-Meulenberghs, F.: Contrasting perspectives on soil evaporation in soil science and land surface modelling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19707, https://doi.org/10.5194/egusphere-egu26-19707, 2026.

EGU26-19852 | ECS | Orals | SSS6.1

 Resolving Event-Driven Soil Gas Fluxes by Coupling High-Frequency Chamber Measurements with Advection–Diffusion Modeling 

Alex Naoki Asato Kobayashi, Neomi Widmer, Clément Roques, Daniel Hunkeler, Laurel ThomasArrigo, and Philip Brunner

Soil greenhouse gas (GHG) emissions in agricultural, forestry, and other land uses are driven by coupled biological and physical processes. To monitor these fluxes, automatic chamber systems are now widely used as point-scale measurement techniques. Their high-frequency records provide richer observational coverage across meteorological and hydrogeological conditions, thereby improving the accuracy of annual soil carbon budgets.

Despite advances in monitoring, long-term soil carbon models usually focus solely on simulating soil carbon turnover and decomposition, omitting mechanisms of soil gas transport. Although this simplification may be reasonable in the topsoil, sharp changes in soil saturation or other meteorological factors are not necessarily captured, which can lead to underestimating short-term emissions and biasing annual GHG budgets.

We investigated this issue in a pilot site in the agricultural region (Seeland region, Switzerland) where the water table depth was controlled. We simulated a short flooding event and continuously monitored soil gas flux at high frequency. And our results showed a dampening in CO2 soil gas flux for the flooded plot compared to our control plot, which persisted after it was drained. While this decrease in CO2 flux can be partly attributed to a reduction in aerobic microbial activity, the timescale to recovery to background CO2 fluxes can be attributed to other mechanisms, including advection-diffusion gas transport in the unsaturated zone.

To interpret these dynamics, we employed a 1-D model to assess the role of advection-diffusion, including pressure-driven gas transport, during short-term events. Our model couples water, heat, and gas transport with microbially driven CO2 production. We conducted a sensitivity analysis evaluating different soil conditions and event intensities.

Finally, the integration between high-frequency soil gas flux monitoring systems and gas transport in the unsaturated zone helps deconvolute the soil gas flux signal, while improving the accuracy of the soil GHG budget. This will enhance the process understanding, which can support agricultural management strategies to minimize GHG emissions.

How to cite: Asato Kobayashi, A. N., Widmer, N., Roques, C., Hunkeler, D., ThomasArrigo, L., and Brunner, P.:  Resolving Event-Driven Soil Gas Fluxes by Coupling High-Frequency Chamber Measurements with Advection–Diffusion Modeling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19852, https://doi.org/10.5194/egusphere-egu26-19852, 2026.

EGU26-20805 | ECS | Orals | SSS6.1

Damage mechanism and spatial heterogeneity of loess subjected to explosion loading 

Dong Tang, Longsheng Deng, Tong Wang, and Wenjie Zhang

The accelerated urbanization of the Chinese Loess Plateau has promoted the wide application of engineering explosion on the rapid excavation in loess regions. However, blasting in loess typically causes the various degrees of damage and failure to the remaining soil mass, compromising the bearing capacity and stability of the surrounding loess. Therefore, understanding the damage characteristics and microstructure changes of loess under explosion loading is essential for the construction of explosion projects in loess regions. In this study, the in-situ explosion experiment, dynamic triaxial tests, and micro-computed tomography (μ-CT) technology were employed to reveal the development characteristics of the blasting cavity, explore the dynamic properties of loess following the explosion, and visualize and quantitatively analyze the variation regulations of the loess microstructure. The results indicated that the shape of the blasting cavity was approximated as an ellipsoid. Explosion caused the breakage and rearrangement of particles and aggregates, significantly increasing the compaction of the loess mass, which promoted the evolution of loess dynamics properties towards high dynamic shear modulus and low dynamic damping ratio. In addition, the explosion loading significantly changed the size, number, morphology, and orientation of the loess pores, thereby causing a degradation in the pore network structure, and reducing its connectivity. Based on the spatial differentiation characteristics of the loess microstructure, the explosion zone outside the blasting chamber was divided into broken, plastic, and elastic zone. These findings provide valuable insights into the damage mechanism of loess under blasting loading.

How to cite: Tang, D., Deng, L., Wang, T., and Zhang, W.: Damage mechanism and spatial heterogeneity of loess subjected to explosion loading, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20805, https://doi.org/10.5194/egusphere-egu26-20805, 2026.

EGU26-21721 | ECS | Posters on site | SSS6.1

Biochar effects on soil hydraulic properties: high-resolution analysis for contrasting soil textures 

Jannis Bosse, Magdalena Sut-Lohmann, Wolfgang Durner, and Sascha C. Iden

Biochar amendment is widely promoted as a means to sequester carbon while improving soil physical properties. Its hydraulic effects depend strongly on particle size and application rate. Available studies mainly focus on enhanced water retention in sandy soils. Studies that include fine-textured soils and quantify effects on unsaturated hydraulic conductivity remain limited, hampering the development of reliable management strategies. Here, we present the effects of biochar addition on the soil hydraulic properties (SHP) of two agricultural topsoils with contrasting textures. Water retention and hydraulic conductivity of a loam and a loamy sand were measured after amendment with wood-derived biochar of three particle sizes (<0.5, <2, and <10 mm) applied at three dosages (1, 2 and 4 wt.%). All samples were packed under identical force and characterized over the full moisture range using the simplified evaporation method, complemented by saturated conductivity measurements and dew-point measurements of dry-range water retention. A comprehensive soil hydraulic model incorporating adsorption and film flow was fitted to all data, enabling systematic analysis of how biochar size and amount affect hydraulic behavior. Relative to the controls, all biochar treatments increased porosity and saturated water content. Saturated hydraulic conductivity increased by up to 200% for the loam but decreased for the sand. In the loam, biochar application improved air capacity by up to 6 vol.% but had no effect on plant-available water. In contrast, biochar quantity and particle size had no effect on the air capacity of the sand, but increased its available water content by up to 3 vol.%. Higher biochar application rates were strongly associated with lower air-entry values, reduced bulk density, and a broader pore-size distribution. This indicates a shift toward smaller pores in the loamy sand and larger pores in the loam. Smaller biochar particles slightly increased unsaturated hydraulic conductivity between 100 and 300 cm suction for both soils, but reduced water retention in the sand at suctions greater than 100 cm compared to coarser biochar. Overall, our findings demonstrate a substantial influence of biochar on soil hydraulic conductivity and water retention, with effects being stronger in coarse-textured soils and more sensitive to application rate than to particle size.

How to cite: Bosse, J., Sut-Lohmann, M., Durner, W., and Iden, S. C.: Biochar effects on soil hydraulic properties: high-resolution analysis for contrasting soil textures, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21721, https://doi.org/10.5194/egusphere-egu26-21721, 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.

Reliable soil moisture estimation is challenged by sparse in-situ networks, inconsistencies across satellite products, and structural limitations in simplified land-surface models. This study develops a machine learning assisted calibration framework for pyWBM, a Python implementation of the University of New Hampshire Water Balance Model, to generate improved historical reconstructions and ensemble projections of root-zone soil moisture for counties across Illinois. We integrate in-situ observations from nine Illinois State Water Survey stations with satellite and reanalysis soil moisture estimates from Soil Moisture Active Passive Level 4 Carbon Product Version 7 (SMAP L4C Version 7) and North American Land Data Assimilation System Phase 2 (NLDAS-2) model outputs (VIC, NOAH, MOSAIC). Meteorological forcing is obtained from Gridded Surface Meteorological Dataset (GRIDMET) for calibration and Localized Constructed Analogs Version 2 (LOCA2) for future projections. Calibration targets multiple key parameters that control storage dynamics and partitioning processes including available water capacity, wilting point, drying coefficient, runoff shape factor, and Potential Evapotranspiration (PET) scaling coefficients. Using JAX-based automatic differentiation, we evaluate thirteen loss functions and identify three, Root Mean Square Error (RMSE), Outer 50 Percent Root Mean Square Error (Outer50RMSE), and Kiling-Gupta Efficiency (KGE), as the most informative based on performance over the full record, the driest five days per year, and the wettest five days per year. Parameter comparisons reveal robust differences between calibration sources: wilting point is systematically higher when calibrated with in-situ data, even when the ensemble is expanded across alternative loss functions. In contrast, available water capacity does not show a consistent separation between satellite- and in-situ-based estimates. Residuals exhibit slight seasonality, with the Outer50RMSE trained models showing the largest variance. To assess ensemble coverage, we introduce an ensemble coverage metric defined as the ratio between the intersection of ensemble spread and observed soil moisture relative to the observed range. In 6 of 9 counties, satellite-based calibrations produce higher coverage, indicating that multi-source calibration can better represent the overall distribution of soil moisture despite the limited temporal record of in-situ data. Projection ensembles generated using seven-year versus twenty-year calibration windows exhibit consistent drying signals across counties, and longer calibration periods reduce the spread of extreme projections while stabilizing parameter distributions. Overall, the results show that integrating in-situ, satellite, and reanalysis datasets with machine learning–enabled calibration improves model performance, enhances ensemble robustness, and provides more defensible future projections. However, the model still struggles to capture abrupt soil moisture declines and seasonal transitions, highlighting ongoing limitations in simplified water balance models when confronted with extreme hydrologic variability. The framework developed here offers a scalable pathway for generating county-scale soil moisture projections to support drought monitoring, agricultural decision-making, and climate resilience planning.

How to cite: Alam, T., Avila, T., Lafferty, D., Ford, T., and Sriver, R.: Machine Learning Assisted Calibration of pyWBM Using In-Situ, Satellite, and Reanalysis Soil Moisture Data for High Resolution Soil Moisture Ensemble Projections, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-357, https://doi.org/10.5194/egusphere-egu26-357, 2026.

Climate change is intensifying soil moisture variability, atmospheric evaporative demand, and salinity intrusion in agricultural landscapes, creating new challenges for sustainable food production. Understanding how soil hydrology and plant physiological stress interact under these conditions is essential for designing resilient irrigation strategies. This study presents a hydro-physiological assessment of wheat and maize grown under controlled combinations of soil salinity and deficit irrigation, and introduces an Artificial Neural Network (ANN) based Crop Water Stress Index (CWSI) model for real-time decision support in semi-arid farming systems of northern India.
Field experiments (2023–2025) were conducted to measure canopy temperature, air temperature, relative humidity, vapor pressure deficit (VPD), and soil moisture under varying salinity (EC levels) and irrigation regimes. These data were used to develop whole-season and stage-specific ANN models capable of capturing non-linear interactions between soil hydrology, crop physiology, and atmospheric demand. The ANN-based CWSI successfully distinguished mild-to-severe stress transitions and detected early-stage water stress acceleration during periods of high VPD, indicating a propensity toward flash drought development under combined salinity–moisture constraints.
Results show that salinity amplifies crop water stress by reducing effective root-zone moisture availability, leading to higher canopy–air temperature gradients and elevated CWSI values even under moderate irrigation. Stage-specific ANN models achieved strong performance (R² = 0.87–0.94), particularly during flowering and grain filling, where hydrological stress most affects yield. The framework demonstrates how data-driven CWSI modeling can translate complex soil–plant–atmosphere interactions into actionable irrigation insights for farmers.
This work highlights a scalable approach to precision irrigation scheduling, enabling reduced water use without compromising crop health in regions vulnerable to hydrological extremes and sociohydrological pressures. By linking soil hydrology, irrigation management, and physiologically informed stress indicators, the study contributes to sustainable food production strategies in a global climate change context.

How to cite: Dandotia, P. K. and Kotnoor Suryanarayanarao, H. P.: Hydro-Physiological Controls of Crop Water Stress Under Salinity and Deficit Irrigation: An ANN-Based Framework for Sustainable Irrigation Management in a Changing Climate, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-772, https://doi.org/10.5194/egusphere-egu26-772, 2026.

EGU26-1500 | PICO | HS8.3.1

Design and deployment of a multi-platform soil moisture monitoring network 

Felix Thomas, Friedrich Boeing, Julian Schlaak, Solveig Landmark, Rebekka Lange, Daniel Altdorff, Jan Bumberger, Andreas Marx, Peter Dietrich, Falk Böttcher, Rainer Petzold, Kerstin Jäkel, and Martin Schrön

The MOWAX project investigates monitoring- and modelling concepts as a basis for the assessment of the water budget in Saxony. It operates a dense, multi‑platform soil moisture observation network in collaboration with the German Weather Service (DWD), Sachsenforst, TU Dresden and regional authorities.

The network was designed to represent the dominant landscape properties influencing the water budget in Saxony, including land use, natural areas, soil types, and climatic conditions. It combines up to 10 area‑representative Cosmic Ray Neutron Sensing (CRNS) stations and novel mobile platforms, namely Rail-CRNS (continuous measurements from sensors on trains). We describe our standardized sensor deployment and calibration protocols, automated quality control procedures, and methods for integrating our observations into the modelling framework using the new UFZ timeseries infrastructure. After more than one year of effort, we report on advancements and experiences in pursuing our goals. Based on our strong collaboration with existing observatories and data management infrastructures we are maximizing the utility of ongoing CRNS data for our purposes by establishing a new sensor network.

One of the primary objectives is to enhance and validate the mesoscale Hydrologic Model (mHM) for Saxony by providing continuous, quality‑controlled soil moisture time series. Further, we aim to provide a near-real-time visualization of our observations and model outputs and deliver a valuable data basis that can be used by authorities to support management decisions and urgent actions.

MOWAX is funded by the European Regional Development Fund (EFRE) and by tax revenue on the basis of the budget approved by the Saxon state parliament (funding code 100702604).

How to cite: Thomas, F., Boeing, F., Schlaak, J., Landmark, S., Lange, R., Altdorff, D., Bumberger, J., Marx, A., Dietrich, P., Böttcher, F., Petzold, R., Jäkel, K., and Schrön, M.: Design and deployment of a multi-platform soil moisture monitoring network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1500, https://doi.org/10.5194/egusphere-egu26-1500, 2026.

The electrical properties of materials, specifically dielectric permittivity (ε) and electrical conductivity (σ), are of interest in a wide variety of applications (e.g. agriculture). For example, in porous media such as soil, ε is strongly correlated with water content, and dielectric sensors are routinely employed to measure soil moisture. Soil moisture sensing technologies have been available in the market for decades, including Time Domain Reflectometry (TDR), Impedance Sensors, Capacitance and Frequency Domain Reflectometers (FDR). These sensors all measure the apparent dielectric permittivity εa, which is a function of both the imaginary dielectric permittivity (εi) and εr. Sensor technology needs to be developed to measure both εr and εi in order to overcome the impact of salts on water content measurements and take the next technological step forward. A new method, the four-voltmeter method (4VM) is a complex dielectric sensor that determines both the εr and εi by measuring voltage amplitudes at multiple circuit nodes. The 4VM improves dielectric permittivity measurements under saline conditions by combining multiple independent admittance estimates to account for conductivity-induced errors, avoid loss of sensitivity, and maintain accuracy across a wide range of salinities. The goal of this project is to assess the performance of 4VM in a sandy soil across a range of salinities up to 50 dS/m and assess its true performance.  

How to cite: Rivera, L., Fakhouri, S., and Chambers, C.: Measuring soil moisture and dielectric permittivity in saline environments: Exploring the limits of Complex Dielectric Through Intersections Technology, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2223, https://doi.org/10.5194/egusphere-egu26-2223, 2026.

EGU26-6582 | PICO | HS8.3.1

Summer drying of soils in Switzerland: Insights from the SwissSMEX network 

Martin Hirschi, Dominik Michel, Dominik L. Schumacher, Wolfgang Preimesberger, and Sonia I. Seneviratne

Notably drier summers and more frequent droughts were reported in Switzerland in the last decades. We analyse these drying trends based on the comprehensive network of in situ soil moisture measurements from the Swiss Soil Moisture Experiment (SwissSMEX), which as of now covers 15 years. We document recent measures that have been taken to secure the SwissSMEX network and to ensure the continuity of its long-term soil moisture timeseries. The analysis focuses on trends in summer and summer half-year anomalies of vertically integrated soil water content and investigates the robustness of the recent drying based on different sets of Swiss Plateau stations. Furthermore, the SwissSMEX-based trends are compared with those from soil moisture of a widely used land reanalysis product (ERA5-Land) and of a merged passive microwave satellite product (European Space Agency Climate Change Initiative ESA CCI).

There is good agreement between the temporal evolution and the drying tendency of SwissSMEX in situ soil moisture based on different sets of Swiss Plateau stations. Comparisons with ERA5-Land and ESA CCI reveal a consistent evolution of soil moisture across the three independent datasets. Summer drying tendencies over the common 2010–2025 period amount to ‑11 mm/decade for ERA5-Land and ESA CCI, and to ‑14 mm/decade for SwissSMEX. While most drying trends are not statistically significant over this short span, ERA5-Land shows significance when extending the analysis period. The findings underscore the need for continued soil moisture monitoring in Switzerland for further investigation of long-term drying trends.

How to cite: Hirschi, M., Michel, D., Schumacher, D. L., Preimesberger, W., and Seneviratne, S. I.: Summer drying of soils in Switzerland: Insights from the SwissSMEX network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6582, https://doi.org/10.5194/egusphere-egu26-6582, 2026.

EGU26-8959 | ECS | PICO | HS8.3.1

From raw measurements to indicators: workflows for quality-controlled soil moisture monitoring in Austria 

Florian Darmann, Verena Jagersberger, Jutta Eybl, Korbinian Breinl, Peter Strauss, and Thomas Weninger

Understanding soil water dynamics is crucial for hydrological assessments in Austria’s intensively used landscapes. Reliable soil moisture observations support the understanding of vadose zone processes and can be used to assess infiltration capacity during heavy rainfall events, as well as to evaluate water availability during dry periods. However, sensor-related uncertainties and data quality issues limit the application of soil moisture monitoring networks in hydrological modelling, despite their long-term operation and broad relevance.

The Austrian Hydrological Service operates a nationwide monitoring network measuring soil water content, matric potential, and soil temperature at multiple depths across diverse climatic and land-use conditions. These long-term observations provide an important basis for climate trend analysis and the development of water management strategies. The sustainable use of such datasets depends on robust data management and quality assurance procedures.

This study focuses on establishing a standardized and reliable workflow for transforming raw soil water measurements into publicly accessible indicators. This includes the development of quality control and data processing procedures for Austria’s soil moisture monitoring network. Automated and semi-automated routines are used to identify measurement errors related to sensor problems, signal drift, and implausible temporal behaviour. These routines are complemented by systematic data correction procedures. The resulting quality-controlled time series form the basis for deriving soil water indicators (e.g. the Soil Water Index) and enable near-real-time visualization within the national hydrological portal eHYD.

The presented workflow improves the consistency, reliability, and accessibility of long-term soil moisture observations by providing a framework for quality control and data processing. This approach is transferable to other soil moisture monitoring systems with similar challenges regarding data quality, long-term maintenance, and operational use.

How to cite: Darmann, F., Jagersberger, V., Eybl, J., Breinl, K., Strauss, P., and Weninger, T.: From raw measurements to indicators: workflows for quality-controlled soil moisture monitoring in Austria, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8959, https://doi.org/10.5194/egusphere-egu26-8959, 2026.

Authors: Boquera, Lola ; Janeras, Marc ; Lladós, Agnès ; Portell, Xavier and Vicens, Marc

Institut Cartogràfic i Geològic de Catalunya. Parc de Montjuïc 08038, Barcelona, Spain. https://www.icgc.cat/

  XMS-Cat is a soil moisture observation network implemented by the Cartographic and Geological Institute of Catalonia (ICGC) to characterize climatic conditions and soil moisture throughout Catalonia. Each station in the network measures soil temperature and volumetric water content at several depths (typically 5, 20, 50, and 100 cm), as well as atmospheric variables such as rainfall, air temperature, humidity, and solar radiation. The network currently provides high-quality, open-access data for farmers, land managers, and scientists (Soil monitoring network ICGC website:  https://visors.icgc.cat/mesurasols/#9.67/42.4378/0.7495).

While volumetric water content measured by XMS-Cat sensors is a quantitative measure of soil moisture, shallow landslides triggered by rainfall are more closely related to the soil water energy state, which can be better assessed using water potential sensors. Consequently, in 2023, an experimental phase was initiated in which new XMS-Cat stations were supplemented with both types of sensors.The purpose of this enhancement in addition to deepening knowledge of soil water status is threefold: (1) strengthening soil-related hazard assessment, such as slope stability,(2) improving characterization of the vegetation water stress; and (3)introducing data redundancy to enhance network resilience.

This contribution provides further details of the network reconfiguration and the initial studies conducted.

Keywords: soil moisture, in situ monitoring, network, volumetric water content, water potential, agriculture, vegetation water stress, slope stability, Landslide hazard.

How to cite: Boquera, L.: Enhancing the Catalan Soil Moisture Observation Network  (XMS-Cat): from agricultural and climatic applications to hazard assessment.  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9319, https://doi.org/10.5194/egusphere-egu26-9319, 2026.

EGU26-12085 | ECS | PICO | HS8.3.1

Assessing Spatial Variability of Soil Moisture Across an Erosion-Prone Agricultural Hillslope  

Doğa Yahşi, Svenja Hoffmeister, Mirko Mälicke, Núria Martínez-Carreras, Jean François Iffly, and Erwin Zehe

Soil moisture is a critical state variable in hydrological systems, acting as both an initial and a boundary condition for physically based hydrological models. Its spatial and temporal variability strongly influences the partitioning of rainfall into infiltration, overland flow and subsurface runoff, which regulates the magnitude, timing and threshold behaviour of extreme events such as flash floods and soil degradation. However, the extensive and multiscale variability of soil moisture has challenged hydrological scientists for over two decades. A common approach to address this issue is to perform distributed point sampling of soil moisture and apply geostatistical methods to analyze spatial relationships and patterns, perform interpolations and provide uncertainty estimates for predictions.

In this study, we aim to quantify the spatial variability of soil moisture at the hillslope scale, as this variability is a key factor controlling hydrological responses and erosion dynamics. The research area is an agricultural hillslope in the Attert River Basin, Luxembourg, where severe erosion occurs year-round on agricultural parcels due steep slopes and extreme rainfall events. A nested cluster sampling design was implemented to cover as much area as possible and to represent a wide range of distance classes to perform geostatistical analysis.

Two soil moisture campaigns were conducted under wet and dry conditions. Soil moisture was measured at 110 cluster points using Time Domain Reflectometry (TDR), which records dielectric permittivity and converts it into volumetric water content using general onboard calibration equations, selected according to soil texture. While these factory calibrations are widely used, they can introduce errors when applied to soils with specific hydraulic properties or textures. Therefore, 15 soil samples (3 per cluster) were collected for gravimetric determination of soil moisture to validate the TDR measurements.

During both campaigns, the TDR measurements revealed a negative bias compared to the gravimetric measurements. Empirical variogram models were fitted for both datasets, with and without the data correction for the bias. The wet case, in comparison to the dry case, exhibited a shorter effective range (~145 m) and a higher nugget-to-sill ratio (~0.4), indicating weaker spatial correlation and a larger relative contribution of small-scale variability. In contrast, the dry case showed a longer effective range (~190 m) and a lower nugget-to-sill ratio (~0.3) reflecting stronger spatial organization and more coherent soil moisture patterns. These differences arise because under wet conditions, increased hydraulic connectivity and redistribution promote local-scale variability and reduce large-scale spatial organization. On the other hand, drier conditions enhance the influence of soil texture, rooting depth and evapotranspiration patterns that operate over larger spatial scales.

How to cite: Yahşi, D., Hoffmeister, S., Mälicke, M., Martínez-Carreras, N., Iffly, J. F., and Zehe, E.: Assessing Spatial Variability of Soil Moisture Across an Erosion-Prone Agricultural Hillslope , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12085, https://doi.org/10.5194/egusphere-egu26-12085, 2026.

EGU26-13497 | ECS | PICO | HS8.3.1

Low-cost soil moisture monitoring: experiences from a technology transfer project for small farms  

Lorenzo Gallia, Giacomo Tavernelli, Dario Vallauri, Cristina Allisiardi, Franco Tesio, and Alessandro Casasso

The importance of irrigation water management has increased in recent years with the declining summer availability due to climate change, especially for surface waters. The diffusion of pressure irrigation systems has led to higher water efficiency exploiting a demand-based irrigation, overcoming the turn-based limitation of classical flood irrigation. GUARDIANS project (https://guardians-project.eu/), funded by the Horizon Europe program and involving 22 partners from 9 countries, has the goal to transfer this approach shift in the context of small farms, developing and demonstrating IT technologies in several study areas. One of these case studies is the irrigation reservoir of Rivoira (Boves, Piedmont, NW Italy), built in 2017 and having a capacity of 42000 m3. The reservoir is connected to a pressure irrigation network serving about 300 ha of cropfields mainly owned by small farmers.

To improve water management in the study area based on actual soil moisture readings, low-cost sensors were tested for ground-based measurement of volumetric water content (VWC). Their affordability makes them suitable for small farms, while remote data transmission enables continuous monitoring across multiple points within the same field.

These sensors, however, present several challenges. Calibration procedures that balance accuracy and simplicity are essential: for example, the choice is between calibrating each sensor or deriving a calibration formula that applies to all of them, or between calibrating sensors for each soil type or with a formula that works for all types. Furthermore, practical considerations for field installation and reliable long-term data transmission are crucial. Measurement quality must also be carefully evaluated, making sensor redundancy important to compensate for devices that may go offline or produce anomalous readings over time.

This work focuses on operational challenges and solutions adopted during calibration, installation, and data management of low-cost soil moisture sensors in the context of seven small farms. The comparison with meteorological data and recorded irrigation events makes it possible to check the performance of the sensors installed during the previous irrigation season, thereby allowing conclusions to be drawn about the reliability of sensors. In particular, the field monitoring campaign revealed similar dynamic behaviour among sensors, which correctly responded to irrigation and rainfall events; however, significant offsets in their absolute VWC values were observed. These discrepancies may be attributed to spatial heterogeneity in field VWC distribution, as well as to sensor drift over time, and deserve particular consideration.

Overall, low-cost sensors can play an important role in improving irrigation management, but several operational challenges need to be addressed to fully exploit their potential.

This study is carried out within the framework of the GUARDIANS project, funded by the European Union through the Horizon Europe Programme - Farm2Fork (Grant Agreement n. 101084468).

How to cite: Gallia, L., Tavernelli, G., Vallauri, D., Allisiardi, C., Tesio, F., and Casasso, A.: Low-cost soil moisture monitoring: experiences from a technology transfer project for small farms , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13497, https://doi.org/10.5194/egusphere-egu26-13497, 2026.

EGU26-13748 | ECS | PICO | HS8.3.1

A long-term soil moisture monitoring network in Twente, the Netherlands: observations, applications, and perspectives 

Franziska Tügel, Paul Vermunt, Murat Ucer, Friso Koop, Filippo Signora, and Christiaan van der Tol

The ITC Faculty at the University of Twente operates a soil moisture monitoring network consisting of approximately 20 stations that continuously measure volumetric soil water content and soil temperature at up to five depths between 5 and 80 cm. The network was originally established in 2009; over time, several stations have been removed, while others have been added. Its initial purpose was to support the calibration and validation of satellite-based soil moisture products. Recent applications use soil moisture and groundwater monitoring to support adapted water management practices, including adjustable weirs and controlled drainage. For this purpose, supplementary soil moisture stations have been installed in smaller clusters within projects conducted in collaboration with local farmers and the regional water authority Vechtstromen. The quality-checked dataset from 2009-2020 has been published by van der Velde et al. (2023) and also added to the International Soil Moisture Network (ISMN). Furthermore, real-time and historical soil moisture data contribute to the Dutch drought portal. Recently, the soil moisture network has been integrated into the development of a larger multi-sensor infrastructure at the ITC, supported by the NWO-funded Sectorplan in Earth and Environmental Sciences.

The collected data will be analyzed to investigate long-term trends, responses to meteorological extremes, and spatial variability in soil moisture across the Twente region. Furthermore, data from soil moisture, meteorological, groundwater, and additional sensors, together with remote sensing observations, will serve as calibration and validation data for an integrated hydrological model. This framework aims to investigate the effects of local agricultural water management practices on water fluxes and water balance components, such as evapotranspiration, groundwater recharge, and surface runoff, and to scale up field-level adaptation measures and their effects to the regional scale. Insights from these investigations are expected to support the identification of sustainable and resilient water management practices from field to regional scales, helping to better cope with increasing water-related challenges such as droughts and flooding.

References: van der Velde, R., Benninga, H.-J. F., Retsios, B., Vermunt, P. C., and Salama, M. S.: Twelve years of profile soil moisture and temperature measurements in Twente, the Netherlands, Earth Syst. Sci. Data, 15, 1889–1910, https://doi.org/10.5194/essd-15-1889-2023, 2023.

How to cite: Tügel, F., Vermunt, P., Ucer, M., Koop, F., Signora, F., and van der Tol, C.: A long-term soil moisture monitoring network in Twente, the Netherlands: observations, applications, and perspectives, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13748, https://doi.org/10.5194/egusphere-egu26-13748, 2026.

High-resolution soil moisture data is a critical component for understanding the hydrological cycle and establishing climate adaptation strategies, particularly in the complex mountainous terrains of the Far East Asian region. Recognizing the significance of this data within the southern part of the Korean Peninsula, the Korea Institute of Hydrological Survey operates in-situ soil moisture monitoring networks to provide standardized, high-quality hydrological data. Located in mountainous regions with long-term operational history, these networks are co-located with evapotranspiration and streamflow stations, facilitating efficient and integrated water balance studies.

To ensure high data reliability for global research applications, KIHS implements a multi-stage quality control (QC) framework for its SM datasets. We have developed an automated outlier detection system based on the International Soil Moisture Network (ISMN) protocols to identify and filter physical anomalies such as spike, break and constant values. Furthermore, to provide continuous data, KIHS utilizes a hybrid framework of statistical methods and machine learning algorithms for gap-filling. This framework integrates CDF Matching, Kalman Filter, and SARIMAX with non-linear models like Random Forest and KNN, ensuring robust and continuous time-series data even under challenging field conditions.

These high-quality datasets are shared internationally through ISMN and are highly recommended for the calibration and validation of satellite products such as SMAP and Sentinel, particularly during the non-frozen period from April to November. The objective of this presentation is to present KIHS's soil moisture monitoring networks and QC methodologies and to demonstrate the academic significance of soil moisture observation stations in the Korean Peninsula.

keywords : soil moisture, the Korea Peninsula, mountainous terrain, monitoring networks, long-term operation, QC frameworks

How to cite: Lee, Y. J., Kim, K. Y., and Kim, C. Y.: Enhancing Soil Moisture Data Reliability in South Korea: Advanced Quality Control and Ensemble Gap-filling of the KIHS Network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16168, https://doi.org/10.5194/egusphere-egu26-16168, 2026.

EGU26-18942 | ECS | PICO | HS8.3.1

Establishment of the Israeli Soil Moisture Monitoring Network 

Dotan Perlstein, Ehud Strobach, and Ori Adam

Establishment of the Israeli Soil Moisture Monitoring Network

Dotan Perlstein [a, b], Ehud Strobach [a], Daniel Kurzman [a], Ori Adam [b], Marc Perel [c] 

a Soil, Water and Environmental Sciences, Agricultural Research Organization, Rishon Letzion, Israel

b Institute of Earth Sciences, The Hebrew University, Jerusalem, Israel

c Agrometeorological Division, Israel Ministry of Agriculture

Volumetric water content in unsaturated soil is a complex state variable, highly significant to both agriculture and climate science, but until recently available only in low temporal and spatial resolution. However, recent simplified sensor technologies, advances in digital data logging and telemetry, the emergence of data‑driven analysis methods, together with increasing demand for ground‑truth observations, catalyzed the establishment of soil water monitoring networks worldwide.

Recently, one such network has been established in Israel, through collaboration between the Agricultural Research Organization, Volcani Institute and the Agrometeorological Division of the Israeli Ministry of Agriculture, integrated within the existing infrastructure of above-ground, in-situ meteorological stations. Locations for the soil monitoring stations were selected based on geographic considerations, representing all major soil types and heterogeneous climatic conditions in Israel.

At present, there are 28 operational soil monitoring stations, equipped with TDR‑based soil probes installed at four depths: 10, 30, 70, and 150 cm below ground surface, providing 10‑minute measurements of volumetric soil water content and soil temperature. To minimize disturbance‑induced bias, sensors are installed into undisturbed vertical soil faces exposed by mechanical excavation. Procedures for automated quality control, data validation and user‑interface development are currently underway.

Preliminary results are presented from several stations. For instance, the Mevo Horon station, characterized by a soil profile of mixed carbonate bedrock and rendzina soils, has accumulated more than two years of continuous observations. The data indicate that soil water content at 10 cm depth exhibited more than ten wetting–drying cycles during the 2023–2024 winter season, whereas only a single infiltration event was detectable at 30 and 70 cm depths. At 150 cm depth, soil water content showed no discernible response to the annual hydrological cycle. Diurnal soil temperature signal is clearly observed only at 10 cm depth, with the diurnal thermal wave substantially attenuated even at 30 cm depth, throughout the year.

How to cite: Perlstein, D., Strobach, E., and Adam, O.: Establishment of the Israeli Soil Moisture Monitoring Network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18942, https://doi.org/10.5194/egusphere-egu26-18942, 2026.

EGU26-20609 | ECS | PICO | HS8.3.1

Own the Data, Understand the Land: Citizens as Key Players in Soil Moisture Monitoring? 

Hannah Sachße, Daniel Diehl, Nikolaus Baumgarten, Elgin Hertel, Frederick Büks, and Björn Kluge

Climate change is increasing both the duration of dry periods and the intensity of precipitation events, yet dense, long-term soil moisture records - particularly in rural areas - remain scarce. These records are necessary to understand regional water balances, validate remote sensing data and hydrological models, and provide information for drought-resistant land management. Wassermeisterei is a citizen-led soil moisture monitoring network in the Fläming region around Potsdam and Berlin, Germany. It provides residents with low-cost sensors to continuously measure soil moisture at four depths in the topsoil and subsoil across a growing network of over 70 sites. Participants receive structured education (courses, hands-on-workshops, and online materials) and are supported to install and maintain sensors in their communities (e.g., agricultural land, grassland, gardens, forests).  A real-time LoRaWAN network feeds monitored data into a collaboratively developed, interactive public water map, making soil moisture data accessible and actionable for local communities and stakeholders. Through community building, shared data analysis, and practical resources for replication, the bottom-up citizen science project promotes local responsibility, closes observation gaps in a cost-effective manner, and potentially creates a replicable model for other soils and land use contexts. This presentation examines the integration of citizen science data into formal databases and assesses the scientific value of data from the soil moisture network. Furthermore, the possibility of using this information to improve regional climate resilience by providing data on the water balance of different land use types is explored.

How to cite: Sachße, H., Diehl, D., Baumgarten, N., Hertel, E., Büks, F., and Kluge, B.: Own the Data, Understand the Land: Citizens as Key Players in Soil Moisture Monitoring?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20609, https://doi.org/10.5194/egusphere-egu26-20609, 2026.

EGU26-21379 | ECS | PICO | HS8.3.1

Calibration Of CS655 Soil Moisture Sensors Under Sahelian Conditions: Effects Of Moisture And Temperature 

Mouhamadou Lamine Faye, Mouhamed Diedhiou, and Frédéric Do

Long-term in situ observations of soil moisture are essential to understand eco-hydrological processes, in the vadose zone and to provide ground reference for remote sensing, especially in Sahelian Africa where such datasets are poorly available. Since 2019, a dense network of time domain reflectometry sensors (CS655 model, Campbell Scientific) has been continuously monitoring soil moisture at the “Faidherbia Flux” experimental site in Sob, Senegal. The system records high-resolution data across multiple locations and depths, from 10 cm down to 480 cm.

However, these data face particular quality issues representative of sandy soils in semi-arid agroecosystems. The main challenges stem from (1) the limited accuracy of the standard Topp calibration under a narrow range of soil water content dominated by dry soil conditions (2) the influence of strong diurnal thermal fluctuations on dielectric measurement near the soil surface. High accuracy is particularly required when it is expected to process reliable modelling based on retention curves, very steep in the case of sandy soils.

To address these questions, we designed an experimental protocol combining in situ and laboratory calibrations. In situ calibration was performed during three distinct hydrological periods—dry (June), intermediate (January), and wet (October) to cover the full range of soil water natural conditions. The results revealed a strong correlation between CS655 readings and gravimetric moisture values (R² = 0.97), but also a consistent underestimation of actual soil moisture by CS655 sensor.

In the laboratory, undisturbed soil samples were collected from two depths (20 cm and 80 cm), chosen based on contrasting bulk densities likely to influence sensor response and potentially require distinct correction relationships. These samples were subjected to controlled temperature variations (from 25 °C to 45 °C) and progressive moisture levels (from 17% to 0%).  At a reference temperature of 25 °C, a relationship between the sensor readings and the actual soil moisture was first established, resulting in a correction coefficient for water content. This relationship confirmed the underestimation of soil water content by CS655 observed in the field. Then, for each moisture level, the slope of the sensor response to temperature was calculated. The average of these slopes defined a temperature correction coefficient.

Based on this two-step approach, we developed a three-variable calibration model, linking measured soil moisture, actual soil moisture, and soil temperature variations. Applying these corrections to field data significantly improved the accuracy and robustness of the CS655 readings. The systematic underestimation bias was corrected, and temperature-driven fluctuations were substantially reduced, allowing a more reliable interpretation of daily and seasonal moisture dynamics.

These findings highlight the importance of sensor calibration protocols for long-term soil moisture monitoring in our ecosystem type. Our work contributes to global efforts aimed at improving in situ networks and supporting satellite validation and hydrological modeling in arid and semi-arid regions.

How to cite: Faye, M. L., Diedhiou, M., and Do, F.: Calibration Of CS655 Soil Moisture Sensors Under Sahelian Conditions: Effects Of Moisture And Temperature, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21379, https://doi.org/10.5194/egusphere-egu26-21379, 2026.

EGU26-23056 | PICO | HS8.3.1

The International Soil Moisture Network (ISMN): revised flagging strategy and AI assisted quality control 

Wolfgang Korres, Tunde Olarinoye, Dominique Mercier, and Matthias Zink

Soil moisture is a key variable influencing land–atmosphere interactions, hydrological extremes, ecosystem processes, and agricultural productivity. The International Soil Moisture Network (ISMN) provides a global, freely-accessible repository of quality-controlled in situ soil moisture observations to support Earth system science, remote sensing validation, and model development through standardized and traceable data. The ISMN compiles soil moisture time series from a wide range of regional, national, and international monitoring networks. Contributing datasets are harmonized in terms of format, metadata, and temporal resolution and subjected to a uniform, rule-based quality control (QC) procedure to ensure research-ready data.

Each observational data point undergoes thirteen plausibility checks, resulting in flagging data as “good” or “dubious”. These checks fall into three categories: (i) a geophysical range verification, identifying  thresholds exceedances (e.g., soil moisture < 0% Vol); (ii) geophysical consistency checks, comparing observations with ancillary in situ data or NASA’s GLDAS Noah model data (e.g., flagging of soil moisture when soil temperature is below 0°C); and (iii) spectrum-based approaches, using the first and second derivatives of soil moisture timeseries to detect irregular patterns such as spikes, breaks, or plateaus.

In this work, we propose targeted adaptations to the existing QC flagging strategy to reduce false positives, where valid measurements are incorrectly marked as “dubious”. These refinements increase the proportion of data points flagged as “good” by up to 15% for the entire database. Also, we are proposing the revision of several flags which are originally optimized for the validation of remote sensing products to enhance usability across broader scientific applications, while still maintaining their utility for the remote sensing community. Finally, we will introduce an AI based change detection algorithm designed to identify and potentially homogenize structural breaks and impute missing or “dubious” values in soil moisture timeseries, such as those caused by sensor replacements. This would enable the generation of longer, more consistent time series records suitable for statistically robust trend analyses.

How to cite: Korres, W., Olarinoye, T., Mercier, D., and Zink, M.: The International Soil Moisture Network (ISMN): revised flagging strategy and AI assisted quality control, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23056, https://doi.org/10.5194/egusphere-egu26-23056, 2026.

This work presents a new method for interpreting potential geomagnetic field data. It combines the analytical signal method, which is independent of the direction of magnetization, with the two-dimensional continuous shearlet transform (CST). First, the dominant directions of the structural geological features of a given area are estimated using geological data and conventional interpretation methods such as horizontal gradient, Euler deconvolution and wavelet transform. These directions are then used to determine the shearing parameters required for the shearlet transform calculation. The two-dimensional CST is then applied to the amplitude of the analytical signal calculated from potential geomagnetic anomaly field data. Mapped maximas of the amplitude of the shearlet transform for the full range of CST scales enable identification of geological discontinuities. The proposed approach avoids reduction to the pole (RTP), which is often problematic in areas with high remanence. It also effectively attenuates the random noise associated with the analytical signal, thereby improving the mapping of magnetic anomalies. Furthermore, it facilitates structural interpretation in geologically complex environments. This process is particularly useful in mining, oil, and geothermal exploration, representing a significant advance in geomagnetic data interpretation.

How to cite: Ouadfeul, S.-A.: Potential geomagnetic field data interpretation using the analytical signal and the two-dimensional continuous Shearlet transform., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-300, https://doi.org/10.5194/egusphere-egu26-300, 2026.

The Assarag region is located in the northern part of the Ouzellagh-Siroua salient, being a segment of the central
Anti-Atlas basement bulging within the High-Atlas Belt of Morocco. It consists mainly of the Late Ediacaran
Magmatic Suites (LEMS) of the Ouarzazate Group (580-539 Ma). The LEMS comprise high potassic calc-alkalic I type
granitoids that host the Imourkhssen Cu-Mo-Au-Ag porphyry mineralization. The aeromagnetic data from
the Assarag region led to describe structural features in the LEMS based on their magnetic footprints. aeromagnetic
datasets were processed using several transformations including the reduction to pole (RTP), Upward
continuation (UC), Tilt derivative (TD), Center for Exploration Targeting (CET) and Euler deconvolution (ED)
filters. RTP, TD and CET transformations allowed to map NNE-SSW, NNW-SSE and NE-SW trending faults in the
north, in addition to a curved magnetic halo in the southwestern part of the Assarag area. The UC filter subdivided
the Assarag area into two magnetic morpho-structural domains: a northern region with low-magnetic
features, and a southern high-magnetic region with positive curved trending patterns. The ED results match
and support the extracted lineaments. The aeromagnetic data were also processed by a 2D Spatio-Spectral
Feature Extraction and Selection tool (SFES2D) using two-dimensional continuous wavelet transformations
(2D CWT), principal component analysis (PCA) and independent component analysis by kurtosis and negentropy
methods (k-ICA and n-ICA). The PCA results corroborate previously extracted lineaments and highlight a new
ENE-WSW oriented structure. Meanwhile, the CWT allowed us to conclude that NNE, NNW and NE trends are
shallow and emphasized deep NW-SE and ENE-WSW structures in the southern part of the Assarag area. ICA
emphasizes the ENE lineament and matches the previous results. We herein define the deeper ENE trend as a part
of the South Atlas Fault (SAF), which crosscuts the LEMS in the study area. Meanwhile, the shallow NE-SW and
NNE-SSW tectonic features likely served as conduits for the ore-bearing fluids, leading to the Imourkhssen Cu-
Mo-Au-Ag mineralization. Consequently, these directions present a valuable approach for guiding mineral
exploration in the Ouzellagh-Siroua salient, from prospect to regional scales.

How to cite: Ferraq, M., Belkacim, S., Cheng, L.-Z., and Abbassi, B.: Aeromagnetic data from the Assarag area (Ouzellagh-Siroua salient, central Anti-Atlas, Morocco): Implications for the Imourkhssen porphyry mineralization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-450, https://doi.org/10.5194/egusphere-egu26-450, 2026.

This study presents a fully automatic inversion technique for interpreting magnetic anomalies of two-dimensional (2D) listric fault structures with arbitrary magnetisation. Listric faults exhibit curved geometries with steep dips near the surface that decrease with depth. But most studies assume a planar fault geometry to the listric faults, which is rarely valid in reality. Accurately modelling such structures is essential because many sedimentary basins and extensional tectonic settings contain listric faults that significantly influence subsurface geometry. Forward modelling is performed using the equation derived by Ani Nibisha et al. (2021), that computes magnetic anomalies of listric faults in any component (vertical, horizontal, or total), with arbitrary magnetisation directions by incorporating both induced and remanent magnetic components. In the proposed method, polynomial function of arbitrary degree is used to represent the nonplanar fault surface. The coefficients of these polynomials, with structural parameters like depths to the top and bottom of the fault, location of the fault edge, and magnetisation intensity and direction, are estimated directly from the magnetic anomaly profile. The inversion uses Marquardt’s (1970) algorithm for optimisation. With a vertical step approximation, the initial parameters are generated automatically based on certain characteristic anomaly features like maximum and minimum anomaly points, and are updated iteratively until a predefined convergence criterion is satisfied. The misfit between observed and calculated anomalies guides model updates, and the method adaptively adjusts the damping factor to ensure stable convergence. The validity and robustness of the inversion technique are demonstrated through two examples. In the synthetic test, a fifth-degree polynomial is used to describe the fault geometry, and Gaussian noise is added to the computed anomalies for a realistic approach. The inversion successfully reconstructs the geometry, magnetisation intensity, and direction, even when lower-order polynomials (second or third degree) are used, since the optimal degree to define the fault geometry remains unknown with the absence of apriori information about the subsurface during inversion. This demonstrates that the technique can produce geologically reasonable solutions even without precise prior knowledge of the fault’s curvature. This technique is compared with the inversion technique by Murthy et al. (2001), which assumes planar fault surfaces and shows that such simplified models fail to recover realistic structures for listric faults. The method is further applied to real total-field magnetic anomalies from the western margin of the Perth Basin, Australia, which is known for hydrocarbon prospectivity and characterised by deep, curved normal faults. Using a second-degree polynomial, the technique identifies a listric fault with its top near 4 km depth and bottom near 14.8 km, yielding a close fit to observed anomalies with small residuals. The recovered geometry aligns well with seismic observations that reveals the listric nature of the fault (Middleton et al. 1993), reinforcing the reliability of the inversion approach. In contrast, inversion assuming a planar fault plane produces geologically inconsistent results. In conclusion, this technique improves the interpretation of magnetic datasets in regions dominated by extensional tectonics and curved fault structures, offering more realistic subsurface models than traditional planar-fault methods.

How to cite: Nibisha, A. and Vishnubhotla, C.: Interpretation of Magnetic Anomalies of 2D Listric Faults with arbitrary magnetisation: A Polynomial-Based Automatic Inversion Approach, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1015, https://doi.org/10.5194/egusphere-egu26-1015, 2026.

EGU26-1487 | Orals | EMRP2.2

Gravity from exploration to field management 

Vijay P Dimri and Ravi Prakash Srivastava

Gravity surveys are well known for the exploration of frontier basins and understanding of the crustal structures.  Recent advances in gravity instrumentation along with processing and interpretation techniques have significantly improved the accuracy of the gravity surveys. The increased accuracy of the gravity measurements has led to Time Lapse gravity (also known as 4D gravity) monitoring of the Oil/Gas fields, where repeatability of the various gravity surveys at different time intervals are crucial.

Plan is to showcase two examples, one related optimum gridding of land 2-D gravity survey based on the scaling concept from Vindhayan basin of India and another where gravity is efficiently used in a very cost effective way for the field management based on repeated gravity measurements at seafloor (Time Lapse gravity) for subsidence and fluid movement monitoring in North sea.

How to cite: Dimri, V. P. and Srivastava, R. P.: Gravity from exploration to field management, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1487, https://doi.org/10.5194/egusphere-egu26-1487, 2026.

EGU26-3131 | Posters on site | EMRP2.2

Gravimetry across spatial scales – how powerful is gravity? 

Hans-Jürgen Götze and Denis Anikiev

Gravity is a fundamental geophysical method that provides unique insight into subsurface density variations. Its sensitivity spans an exceptional range of spatial scales, from centimetre-scale laboratory experiments and borehole measurements to continental - and global-scale satellite observations. Despite its long-standing application, the practical limits and resolving power of gravimetry across these scales are still not widely appreciated. At regional to global scales, satellite missions such as GRACE and GOCE have transformed our understanding of mass redistribution within the Earth system. They enable the monitoring of ice mass loss, hydrological change, and large-scale mantle processes, achieving microgal (10⁻⁸ m s⁻²) accuracy with spatial resolutions of several hundred kilometres. These capabilities demonstrate gravimetry’s strength in detecting large-scale density anomalies and temporal mass transport. At crustal and reservoir scales, terrestrial and airborne gravity measurements resolve subtle variations related to geological structures, sedimentary basins, and fluid movements. Advanced data processing- such as terrain, Bouguer, and isostatic corrections- improves signal fidelity, while time-lapse relative gravimetry can detect changes associated with e.g. volcanic unrest, groundwater depletion, and reservoir dynamics down to the sub-microgal level. At the smallest scales, absolute gravimeters and emerging quantum sensors push precision further, enabling laboratory-based density determinations and environmental monitoring with unprecedented stability. Increasing resolution, however, introduces challenges related to topographic effects, instrumental drift, and signal ambiguity, requiring robust modelling and/or inversion strategies, and integration with complementary geophysical data. We review representative applications across satellite, regional, and local domains, quantify achievable spatial and temporal resolution, and discuss future perspectives, joint interpretation with magnetic and seismic methods, and the growing role of artificial intelligence in gravity data analysis.

How to cite: Götze, H.-J. and Anikiev, D.: Gravimetry across spatial scales – how powerful is gravity?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3131, https://doi.org/10.5194/egusphere-egu26-3131, 2026.

EGU26-3376 | ECS | Orals | EMRP2.2

High-resolution magnetic, sidescan, and water column constraints on the tectono-magmatic and hydrothermal evolution of Healy submarine volcano, Kermadec arc, New Zealand 

Alessio Bagnasco, Fabio Caratori Tontini, Cornel E. J. de Ronde, Sharon L. Walker, Luca Cocchi, Alessandro Ghirotto, and Egidio Armadillo

Here we present a multidisciplinary, high-resolution investigation of Healy submarine volcano, located in the southern Kermadec arc, New Zealand, combining magnetic, sidescan, and hydrothermal plume datasets to constrain the structure and evolution of its magmatic–hydrothermal system.

Near-seafloor magnetic and sidescan sonar data acquired by the Autonomous Underwater Vehicle (AUV) Sentry have been integrated with shipborne magnetic and gravity measurements, multibeam bathymetry, acoustic backscatter, and hydrothermal plume observations, as well as seafloor imagery and in situ temperature measurements collected by the Pisces V submersible, to develop a detailed geological and geophysical characterization of the volcano.

High-resolution sidescan sonar data reveal fine-scale volcanic and tectonic structures, including lava flow textures, fracture networks, and cone morphology providing context for interpreting magnetic anomalies and hydrothermal plume results. Magnetic ‘lows’ are spatially associated with older, caldera-related structures and demarcate zones of ancient hydrothermal discharge, consistent with the loss of magnetite due to hydrothermal alteration. By contrast, younger basaltic cones emplaced along NNE–SSW-trending lineaments exhibit relatively high magnetization signatures and host the currently active hydrothermal venting, characterized by directly observed low-temperature discharge, while hydrothermal plume data (e.g. turbidity anomalies) suggest the possible presence of higher-temperature venting. Taken together, the spatial distribution of volcanic facies, structural lineaments, magnetization patterns, and hydrothermal activity suggests a temporal evolution in magma emplacement and fluid pathways. This evolution is consistent with a transition from caldera-related, arc-dominated volcanism toward more localized basaltic magmatism exploiting extensional structures, which may reflect the early development of back-arc extension.

Our results highlight the important role of multi-sensor, high-resolution surveys in developing robust conceptual models of submarine volcanic systems, and demonstrate how combined gravity, magnetic, sidescan, and hydrothermal plume investigations are prerequisites for understanding hydrothermal processes and related resources in remote deep-sea environments.

How to cite: Bagnasco, A., Caratori Tontini, F., E. J. de Ronde, C., L. Walker, S., Cocchi, L., Ghirotto, A., and Armadillo, E.: High-resolution magnetic, sidescan, and water column constraints on the tectono-magmatic and hydrothermal evolution of Healy submarine volcano, Kermadec arc, New Zealand, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3376, https://doi.org/10.5194/egusphere-egu26-3376, 2026.

High resolution magnetic surveys of the seafloor have become more ubiquitous in recent times with the broad application of autonomous underwater vehicles (AUV) to seafloor investigation.  AUVs can follow a precise path repeatedly which allows to the possibility of repeated measurements through time. This provides unique insight in what was considered mostly static seafloor magnetic properties. Some examples of dynamic magnetic field include anomalies associated with recent lavas cooling and becoming magnetized, while deep-seated thermal anomalies associated with magma chambers may demagnetize the overlying crust and create a detectable signal at the seafloor if not the sea surface.  We present an update to a temporal magnetic study of Axial seamount in the northeast pacific.  Axial Seamount is active having erupted in 2015, 2011, and 1998. Axial is part of the Ocean Observatory Initiative Regional Cabled Array.  Magnetic field is not monitored but repeat, semi-yearly surveys have been done by AUV Sentry for geodetic purposes which happily also collects magnetic field data. We present recent 2024 results from Axial Seamount as it inflates for a future eruption.

How to cite: Tivey, M.: Temporal Magnetic Surveys using Autonomous Underwater Vehicles, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3598, https://doi.org/10.5194/egusphere-egu26-3598, 2026.

EGU26-6661 | Posters on site | EMRP2.2

Potential field and structural control of a Sn-W rich area, W Iberia (Central Iberian Zone) 

Puy Ayarza, Manuela Durán, Pablo Calvín, Irene DeFelipe, Laura Yenes, Alberto Santamaria, Imma Palomeras, Yolanda Sanchez Sanchez, Mariano Yenes, Ramon Carbonell, and Juan Gomez Barreiro

The Sn-W belt of western Iberia coincides with large-scale magnetic anomalies, namely the Porto-Veira-Guarda and the Central System Magnetic Anomalies (PVGMA and CSMA) challenging the well-known relationship between Sn ores and ilmenite (non-magnetic) granites. In fact, these magnetic anomalies overlap a series of gneiss domes developed in the latest stages of Variscan evolution and often hosting local, but abundant critical mineral ores.  Paradoxically, these domes are cored by non-magnetic granites and their by-products, rising the question about the source of the magnetism.

With the goal of unravelling the relationship between mineralization, tectonics and magnetic anomalies, we have carried out a 50 x 50 km2 ground potential field survey in the Martinamor Gneiss Dome and its surroundings, to the southwest of Salamanca. Results from analytical processing and modelling show that shallow and local magnetic anomalies respond to the existence of highly magnetic, albeit uncommon, Upper-Proterozoic to Ordovician metasediments that are not related to the younger (338-300 Ma) Sn-W mineralization. Contrarily, the ores appear at the non-magnetic core of the dome and are frequently related to high gradient zones within potential field data. The latter coincide with the location of extensional detachments that must have acted as pathways for mineralizing fluids. To the southwest of the study area and at higher depths, conspicuous magnetic maxima coincide with Bouguer gravity anomaly maxima and with high shear-wave velocity anomalies, pointing out to the existence of non-outcropping mafic rocks. These lithologies might be progressively more common at depth and be the source of the long wavelength PVGMA and CSMA.  

The present dataset indicates that, as it has been generally acknowledged, magnetic rocks do not host Sn (and W) mineralization but regardless of this evidence, in western Iberia, there might be a common mechanism that triggers mineralization and magnetization. Constraining the age of the latter is key to further interpret this area.

This research has been funded by project SA066P24 from the JCYL

How to cite: Ayarza, P., Durán, M., Calvín, P., DeFelipe, I., Yenes, L., Santamaria, A., Palomeras, I., Sanchez Sanchez, Y., Yenes, M., Carbonell, R., and Gomez Barreiro, J.: Potential field and structural control of a Sn-W rich area, W Iberia (Central Iberian Zone), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6661, https://doi.org/10.5194/egusphere-egu26-6661, 2026.

EGU26-7486 | ECS | Posters on site | EMRP2.2

Inversion of gravity and magnetic data in the presence of topography using deformable hexahedral elements 

Lahcene Bellounis, Romain Brossier, Ludovic Métivier, Claire Bouligand, and Stéphane Garambois

Potential-field geophysical data are commonly used to image geological structures in areas characterized by strong topographic variations, such as volcanic and rift systems. However, the forward modelling of potential-field data using traditional approaches may inadequately represent strongly varying topography if the physical space is not discretized appropriately, potentially biasing inversion results and subsequent geological interpretations. Recent modeling strategies, such as the use of numerical integration schemes within deformable hexahedral elements coupled with an algorithm for local refinement of the forward modeling mesh, have been shown to improve the modeling accuracy while maintaining a reasonable computational cost [Bellounis et al., Geophys. J. Int., ggag009, 2026]. Building on this previous work, we present the implementation of an inversion framework that is consistent with this numerical approach and assess its performance using a series of synthetic data that have not been corrected for topographic effects. The inversion is performed on models discretized using deformable hexahedral elements where physical properties are represented by 2nd order polynomials defined by their values at grid nodes. We first validate the inversion scheme using a model without topography, before considering a second example that incorporates complex topographic variations representative of the Krafla geothermal system in northern Iceland. These synthetic experiments highlight the challenges introduced by topography in the inversion process and demonstrate the improved integration of topographic information enabled by the proposed discretization and inversion strategy. We further examine the influence of the inverse problem regularization parameters on the recovery of subsurface anomalies, thereby providing insights into the advantages and current limitations of the newly implemented inversion framework.

How to cite: Bellounis, L., Brossier, R., Métivier, L., Bouligand, C., and Garambois, S.: Inversion of gravity and magnetic data in the presence of topography using deformable hexahedral elements, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7486, https://doi.org/10.5194/egusphere-egu26-7486, 2026.

EGU26-8366 | ECS | Posters on site | EMRP2.2

Open-source gravity and magnetic forward model of ellipsoids 

Santiago Soler, Kelly Baker, and Lindsey Heagy

Analytic solutions for the gravitational potential of a homogeneous ellipsoid have existed since the first half of the nineteenth century, while analytic solutions for the magnetic field were developed by the end of the same century. The existence of such analytic solutions allowed geophysicists to use ellipsoidal bodies to approximate complex geological structures and model their respective gravity and magnetic fields. Ellipsoids are of particular interest for modelling ore bodies and structures with high magnetic susceptibilities, since they are the only geometric bodies with analytic solutions for their magnetic field that account for self-demagnetization effects. Nonetheless, modern, easy-to-use, up-to-date, and open-source implementations of these analytic solutions are scarce if non-existent.

We present an open-source Python implementation of the analytic solutions of the gravity acceleration and magnetic field generated by homogeneous ellipsoids with arbitrary rotations. This new code allows users to easily define ellipsoids by their semi-axes lengths, the coordinates of their geometric centers, and three rotation angles. The gravity acceleration and magnetic field they generate can be computed on any point in space, including internal and external points to the bodies, through specific functions for each field. The code supports triaxial, prolate and oblate ellipsoids, including spheres. Users can assign physical properties to each ellipsoid, like its mass density, magnetic susceptibility, and remanent magnetization. The magnetic susceptibility can be a single value for isotropic susceptibility, or a second-order tensor to account for anisotropy. The total magnetization of the ellipsoid is obtained as a combination of the induced and remanent magnetization, accounting for self-demagnetization effects.

This implementation can be used to predict the gravity and magnetic field of any set of ellipsoids for hypothesis testing, survey designing, and stochastic inversions. In future work, we plan to include analytic derivatives of the fields with respect to ellipsoid's parameters, so the code can also be used for deterministic inversions.

The ellipsoid class and their forward modelling functions have been included in Harmonica: an open-source Python package for processing and modelling gravity and magnetic data, part of the Fatiando a Terra project. We followed best practices for its development, including thorough testing and extensive documentation, leading to a robust, well-designed, and well-tested implementation of such analytic solutions.

How to cite: Soler, S., Baker, K., and Heagy, L.: Open-source gravity and magnetic forward model of ellipsoids, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8366, https://doi.org/10.5194/egusphere-egu26-8366, 2026.

Mapping crustal thermal structure is fundamental to studies of lithospheric rheology, tectonic evolution, and deep geothermal resource assessment. Curie point depth (CPD) estimates derived from magnetic anomalies are commonly used to infer geothermal gradients, but many approaches remain sensitive to simplifying assumptions about magnetization. Here, a computationally efficient, spatial-domain framework is developed to invert CPD topography by representing the CPD as an effective magnetization-contrast interface and computing its magnetic response using Cauchy-type surface integrals. This formulation replaces three-dimensional volume integration with a two-dimensional surface integral while preserving the governing potential-field physics, which facilitates high-resolution forward modelling and regularized interface inversion. Synthetic experiments are conducted to evaluate numerical accuracy and inversion robustness. The method is applied to magnetic anomalies over the Gonghe Basin on the northeastern Tibetan Plateau, a high-temperature geothermal region. The inverted CPD is interpreted as an effective magnetic-thermal boundary conditional on the assumed susceptibility model, and is compared with results from spectral techniques, equivalent-source reconstructions. Finally, the CPD constraints are integrated with independent geophysical and geological information to construct a three-dimensional temperature model of the Gonghe Basin, which provides quantitative insight into the distribution of thermal anomalies and the likely heat-source characteristics and driving mechanisms.

How to cite: Sun, J. and Liu, S.: Curie Point Depth Inversion From Magnetic Data Using a Cauchy-type Integral Interface Framework: Application to the Gonghe Basin (northwest China), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8781, https://doi.org/10.5194/egusphere-egu26-8781, 2026.

EGU26-9535 | Posters on site | EMRP2.2

The magnetic and electromagnetic integrated geophysical investigation of the Weilasituo tin polymetallic deposit, Inner Mongolia, China 

Shuang Liu, Ronghua Peng, Bo Han, Yajun Liu, Tao Yang, and Zhenhua Zhou

The Weilastuo tin polymetallic deposit is located in the central-southern segment of the Great Xing’an Range, which is an important metallogenic belt of northern China. The Quaternary is widely distributed in the ore district, with the host rocks primarily consisting of migmatitic gneisses and a small amount of Carboniferous quartz diorite. The ore-related intrusive bodies are concealed at depths within the tin-zinc ore district, with the shallowest occurrences reaching approximately 400m below the surface. This study collected the rock samples from the Weilastuo and other districts, and accurately measured the physical properties parameters including resistivity, polarization, magnetic susceptibility, and natural remanent magnetization for over 480 rock samples. The research conducted multi-geophysical explorations and methodological experiments in the Weilastuo ore district, including surface and airborne magnetic exploration, audio magnetotellurics (AMT), and transient electromagnetic (TEM). The 3D magnetic susceptibility and resistivity structure model of the Weilastuo ore district were constructed, providing geophysical constraints for developing geophysical exploration models for shallow cover polymetallic tin deposits of Inner Mongolia, China. This study was supported by project grant no. 2024ZD1001502.

How to cite: Liu, S., Peng, R., Han, B., Liu, Y., Yang, T., and Zhou, Z.: The magnetic and electromagnetic integrated geophysical investigation of the Weilasituo tin polymetallic deposit, Inner Mongolia, China, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9535, https://doi.org/10.5194/egusphere-egu26-9535, 2026.

EGU26-11430 | ECS | Orals | EMRP2.2

From Sharp to Diffuse: How Erosion Level Controls the Architecture of Continental Sutures in the Crust 

Mateusz Mikołajczak, Stanisław Mazur, Randell Stephenson, Christian Schiffer, Piotr Krzywiec, and Jarosław Majka

Continental sutures are fundamental markers of past plate convergence, yet their geological expression varies markedly depending on erosion level and crustal depth. Classical descriptions of sutures emphasize narrow, localized zones characterized by ophiolites, mélanges, arc-related assemblages, and high-pressure metamorphic rocks, often exposed at the surface. However, such features typically reflect shallow-crustal levels of preservation. Here we demonstrate that deeply eroded or buried sutures may lack this diagnostic surface expression and instead form wide, diffuse boundary zones within the middle and lower crust, extending laterally for 100–200 km. This conceptual framework is illustrated with two contrasting examples from Europe: the early Palaeozoic suture between Baltica and Avalonia and the Paleoproterozoic suture between Fennoscandia and Sarmatia within the East European Craton.

The first case examines the German–Polish Caledonides and the Thor Suture separating Avalonia from Baltica. Integration of geological data with reinterpretation of the Basin-9601 deep seismic profile, complemented by newly constructed 2-D forward gravity modelling and regional gravity and magnetic compilations, allows refinement of the crustal architecture across eastern Germany and western Poland. The Caledonian Deformation Front is shown to mark the northern limit of a thin-skinned fold-and-thrust belt, composed of Ordovician metasediments derived from a Caledonian accretionary wedge near Rügen and of deformed foreland-basin sediments incorporated into the orogenic wedge farther east. In contrast, the Thor Suture itself—defined as the thrust of Avalonia’s crystalline basement over Baltica—is located ~120 km farther south, beneath the depocentre of the North German Basin and along the Dolsk Fault Zone in western Poland. At depth, the lower crust of Baltica is underthrust southward to the Flechtingen High and toward the Variscan Rheno–Hercynian suture. This geometry demonstrates that, although the Caledonian suture has a narrow and classical expression in the shallow crust, it broadens downward into a wide lithospheric-scale transition zone, coinciding with mantle lithosphere necking between thick Baltican and thinner Avalonian lithosphere.

The second example addresses the Paleoproterozoic Fennoscandia–Sarmatia Suture (FSS) in eastern Poland. Reassessment of deep reflection seismic data from the PolandSPAN™ survey, combined with 2-D gravity and magnetic modelling and 3-D models of basement depth and crustal thickness, reveals a fundamentally different suture style. Rather than a discrete fault, the FSS is expressed as a 100–120 km wide transitional zone involving the Belarus–Podlasie Granulite Belt and the Okolovo Belt. These domains are characterized by anomalously dense and magnetically susceptible lithologies, interpreted as remnants of arc-related magmatic complexes, mafic igneous suites, and high-pressure metamorphic rocks. Seismic and potential-field data demonstrate that these features continue through the entire crust, indicating a deeply rooted Paleoproterozoic collision that has been subsequently overprinted but not obliterated.

Together, these examples show that sutures preserved at shallow levels are narrow and lithologically distinctive, whereas deeply eroded or ancient sutures are cryptic, broad, and best recognized through integrated seismic and potential-field analyses. At the same time, we acknowledge that differences in Precambrian versus Phanerozoic tectonic regimes—such as lithospheric strength, thermal structure, and strain distribution—may further contribute to the development of especially wide deformation zones in Palaeoproterozoic sutures.

How to cite: Mikołajczak, M., Mazur, S., Stephenson, R., Schiffer, C., Krzywiec, P., and Majka, J.: From Sharp to Diffuse: How Erosion Level Controls the Architecture of Continental Sutures in the Crust, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11430, https://doi.org/10.5194/egusphere-egu26-11430, 2026.

EGU26-11655 | ECS | Posters on site | EMRP2.2

Enhanced Antarctic geothermal heat flow derived from defractal spectral analysis of aeromagnetic data: examples from the Thwaites Glacier and Dome C regions 

Shi Quan Ooi, Fausto Ferraccioli, Pietro Latorraca, Jonathan Ford, Ben Mather, Egidio Armadillo, Joerg Ebbing, Graeme Eagles, Karsten Gohl, Javier Fullea, Massimo Verdoya, and Chris Green

Antarctic geothermal heat flow (GHF) is one of the least constrained basal boundary conditions affecting subglacial hydrology and ice sheet dynamics. Furthermore, the paucity of knowledge about GHF hampers our understanding of the linkages between geodynamic evolution and tectono-thermal conditions in Antarctica.

Here we present the results of enhanced spectral analysis of a new Antarctic aeromagnetic anomaly compilation, conformed at long wavelengths with SWARM satellite magnetic data. We apply manual picking of defractal magnetic power spectra on several different major subglacial lake districts in both West and East Antarctica and compare our results with those obtained using automated workflows implemented in PyCurious. Furthermore, we compare our results with independent GHF estimates from seismology, multivariate-similarity approaches and previous magnetic studies.

We show that in the Amundsen Sea Embayment in West Antarctica manual spectral picking resolves the spatial heterogeneity in GHF anomalies better than automated approaches. We newly define a wide coastal region of relatively lower values corresponding to recently inferred mafic intrusions within this sector of the West Antarctic Rift System and higher GHF in the Byrd Subglacial Basin. This is highly significant as it suggests that elevated GHF may contribute to the onset of enhanced ice flow in the interior of the Thwaites Glacier catchment. Additionally, we find localised GHF anomalies in the area of the Thwaites active lakes that may affect subglacial water availability and promote reduced basal shear stress despite the widespread hard bed conditions related to the occurrence of predominantly crystalline rocks.

In East Antarctica, the manual approach confirms the existence of elevated GHF beneath the Dome C subglacial lake district. However, the anomaly is more linear than previously recognised and better aligned with the trend of major aeromagnetic anomalies interpreted as reflecting extensive Paleo to Mesoproterozoic basement in the sector of East Antarctica. Notably, remarkably similar magnetic anomalies are imaged in formerly contiguous Australia where highly radiogenic igneous provinces significantly enhance GHF.

Overall, we find that the choice of appropriate window sizes and spectral ranges coupled with careful inspection of individual power spectra (including the recognition of outliers) and the choice of defractal parameters is important to better define regional scale heterogeneity in Curie Depth estimates. We also find that incorporating the results of independent seismic, multivariate approaches, and expert knowledge in the geological settings of the different study regions is beneficial to better define the realistic ranges of average Curie Depth and for the conversion from Curie Depth to GHF.

The results of our magnetic studies need to be integrated into thermal modelling frameworks together with the evolving knowledge of crustal and lithospheric properties in Antarctica, including intracrustal heat production and sedimentary basin distribution. This approach will yield improved spatial resolution and accuracy of Antarctic GHF and better understanding of the geological origin and significance of major GHF anomalies.

How to cite: Ooi, S. Q., Ferraccioli, F., Latorraca, P., Ford, J., Mather, B., Armadillo, E., Ebbing, J., Eagles, G., Gohl, K., Fullea, J., Verdoya, M., and Green, C.: Enhanced Antarctic geothermal heat flow derived from defractal spectral analysis of aeromagnetic data: examples from the Thwaites Glacier and Dome C regions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11655, https://doi.org/10.5194/egusphere-egu26-11655, 2026.

EGU26-12390 | Posters on site | EMRP2.2

A Deep Learning Framework for Joint Inversion of Gravity and Magnetic Data 

Xingjian Yan, Shuang Liu, and Mengzhi Lv

Data-driven deep learning inversion of gravity and magnetic data is an emerging technique in obtaining subsurface density and magnetization source distributions. However, the absence of geophysical constraints, inflexibility of structural coupling and oversimplified features of synthetic data restrict the data-driven deep learning joint inversion, outputting models inconsistent with geophysical observations and geological priors. We propose a physics-informed deep learning framework for joint inversion of gravity and magnetic data. The data-driven pre-training is initially utilized by conducting end-to-end supervised training, learning the synthetic features from training dataset. With inverted density and magnetization distributions using pre-trained network, the data misfit and structural losses are calculated for physics-informed fine-tuning of the network. The embedment of physics-informed fine-tuning optimizes data-driven pre-trained network while retaining swift model reconstruction ability, generating models with improved data fitting and model reconstruction of the consistent source regions. The proposed framework is tested on two sets of synthetic examples with different structural homologies and applied to the field data of the Jining iron deposit (northern China). The joint inversion generates density and magnetization distributions for hematite and magnetite and indicates the possibile presence of a regional magnetic basement caused by the high-susceptibility amphibole magnetite quartzite in the Taishan Group. The proposed physics-informed deep learning framework for joint inversion demonstrates the potential of integrating multiple geophysical data and enhances the geophysical consistency in geological modeling.

How to cite: Yan, X., Liu, S., and Lv, M.: A Deep Learning Framework for Joint Inversion of Gravity and Magnetic Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12390, https://doi.org/10.5194/egusphere-egu26-12390, 2026.

EGU26-12493 | ECS | Orals | EMRP2.2

Validation of Drone-Borne Aeromagnetic Surveys Using Multi-Altitude Measurements in Rugged Terrains, Taiwan 

Chung-Wei Chang, Wen-Jeng Huang, Chien-Chih Chen, and Jui-Yu Kao

Geothermal energy is an essential renewable resource whose effective development relies on subsurface structure, particularly in regions with high geothermal potential. Magnetic surveying serves as a fundamental geophysical tool in this context, enabling the identification of concealed intrusions, estimation of source depths, and delineation of buried dykes or faults. While regional airborne campaigns offer efficient coverage, their resolution is often limited by wide survey-line spacing and high flight altitudes. Conversely, ground-based surveys, though detailed, are frequently hindered by rugged terrain and accessibility issues. Drone-borne aeromagnetic surveys address these limitations, providing high-resolution datasets in areas with complex topography.

In this study, we utilized a total-field scalar magnetometer integrated with a multicopter Unmanned Aerial System (UAS) to acquire magnetic measurements. The UAS followed pre-programmed survey lines defined by GPS waypoints and employed terrain-following flight modes at constant altitudes no higher than 120 m above ground level, which are substantially lower than those of conventional airborne surveys and allow measurements to be acquired closer to subsurface magnetic sources. Surveys were conducted at multiple altitudes to calculate vertical magnetic gradients, which serve as essential constraints for modeling subsurface magnetic susceptibility distributions. The data processing workflow comprised spike removal, International Geomagnetic Reference Field (IGRF) correction, and diurnal correction. The processed data were subsequently gridded using the natural neighbor interpolation method to generate magnetic anomaly maps.

Our drone-borne aeromagnetic surveys in volcanic regions have demonstrated strong consistency with existing aeromagnetic datasets while offering significantly enhanced spatial density. This study extends the application of drone-borne aeromagnetic surveying to a metamorphic formation with lava flows. Distinct magnetic anomaly patterns are observed at different flight altitudes. Ongoing research involves the application of computational methods and modeling to analyze these altitude-dependent phenomena and refine the interpretation of subsurface magnetic source distributions.

How to cite: Chang, C.-W., Huang, W.-J., Chen, C.-C., and Kao, J.-Y.: Validation of Drone-Borne Aeromagnetic Surveys Using Multi-Altitude Measurements in Rugged Terrains, Taiwan, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12493, https://doi.org/10.5194/egusphere-egu26-12493, 2026.

Gravity‐Derived Moho Depth of Egypt: Insights from Lithospheric-Scale Gravity Inversion and Comparison with Global Crustal Models

Mohammad Shehata1,2, Hakim Saibi1

1Geosciences Department, College of Science, United Arab Emirates University, 15551, Al-Ain, United Arab Emirates

2Department of Geology, Faculty of Science, Port Said University, Port Said 42522, Egypt

 

Reliable constraints on Moho depth are fundamental for understanding lithospheric structure and tectonic evolution, yet estimates across Egypt and northeastern Africa remain uneven in coverage and resolution. Seismic constraints are restricted to discrete locations, while global crustal models mainly capture long-wavelength features and may not resolve crustal thickness contrasts across different tectonic domains. Here we present a country-scale Moho depth model for Egypt derived from GOCE satellite gravity, providing continuous regional coverage for evaluating tectonically controlled crustal thickness variations.

Bouguer gravity anomalies were computed from GOCE satellite gravity data, complemented where appropriate by terrestrial observations, and corrected for topography, bathymetry, and sedimentary cover. Moho geometry was estimated using frequency-domain Parker–Oldenburg iterative inversion incorporating laterally variable crust–mantle density contrasts derived from the CRUST1.0 model, allowing spatial variations in crustal composition and thickness to be explicitly accounted for (Shehata and Mizunaga, 2022). The resulting Moho model reveals systematic crustal thickness variations that closely correspond to Egypt’s tectonic architecture, with shallow Moho depths (~18–22 km) beneath extensional domains associated with Red Sea rifting, intermediate depths (~28–34 km) in transitional zones such as the Nile Delta and Sinai, and thick crust (>40–43 km) across the Western Desert and southern Egypt. Sharp lateral Moho gradients delineate boundaries between these regimes, indicating localized strain accommodation during rift development. Comparison with CRUST1.0 (Laske et al., 2013), GEMMA (Reguzzoni et al., 2013), and the seismic-based Moho compilation of Tugume et al., 2013) shows overall agreement at long wavelengths, while localized deviations occur in rifted and transitional regions due to differences in data resolution and methodological sensitivity. These results demonstrate that tectonic regime exerts a first-order control on Moho depth beneath Egypt and highlight the value of GOCE-based gravity inversion for improving lithospheric characterization in regions of limited seismic coverage.

References

Laske, G., Masters, G., Ma, Z., Pasyanos, M., 2013. Update on CRUST1. 0—A 1-degree global model of Earth’s crust, in: Geophysical Research Abstracts. p. 2658.

Reguzzoni, M., Sampietro, D., Sansò, F., 2013. Global Moho from the combination of the CRUST2. 0 model and GOCE data. Geophys. J. Int. 195, 222–237.

Shehata, M.A., Mizunaga, H., 2022. Moho depth and tectonic implications of the western United States: insights from gravity data interpretation. Geosci. Lett. 9, 23.

Tugume, F., Nyblade, A.A., Julia, J., Van der Meijde, M., 2013. Crustal shear wave velocity structure and thickness for Archean and Proterozoic terranes in Africa and Arabia from modeling receiver functions, surface wave dispersion, and satellite gravity data. Tectonophysics 609, 250–266.

How to cite: Shehata, M. and Saibi, H.: Gravity‐Derived Moho Depth of Egypt: Insights from Lithospheric-Scale Gravity Inversion and Comparison with Global Crustal Models, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12524, https://doi.org/10.5194/egusphere-egu26-12524, 2026.

EGU26-13520 | Posters on site | EMRP2.2

A Compartmentalized Elevation Model Approach to Terrain Correction in Microgravity Surveys 

Sohail Shahzad and Khan Zaib Jadoon

Microgravity surveying is a high-resolution geophysical technique widely used for detecting subsurface voids, karst features, and localized density variations in engineering, environmental, and geological investigations. However, in complex environments such as steep mountainous terrain, narrow valleys, and urban or built-up areas, standard terrain correction approaches often fail to adequately account for fine-scale topographic variations and man-made structures. These limitations can introduce significant distortions in Bouguer anomalies, particularly at the microGal sensitivity level required for microgravity applications.

This research presents an enhanced terrain correction methodology specifically tailored for microgravity surveys conducted in complex natural and artificial environments. The proposed approach integrates high-resolution elevation data derived from Digital Terrain Models (DTMs), conventional topographic surveys, and 3D LiDAR datasets to construct detailed compartmentalized mass models around each gravity observation point. Surrounding terrain and structures are discretized into three-dimensional volumetric compartments characterized by spatial position, elevation, size, and density. Unlike conventional methods, the approach allows the assignment of variable densities to individual compartments, enabling accurate representation of heterogeneous materials such as rock, air-filled voids, buildings, and structural components.

Gravitational acceleration contributed by each compartment is calculated using Newtonian gravity principles, and the vertical component relevant to terrain correction is extracted and summed to compute station-specific corrections. The methodology is implemented using a database-driven computational framework to efficiently handle the large number of calculations involved. Results demonstrate that the proposed technique significantly improves terrain correction accuracy, effectively capturing the gravitational influence of steep slopes, narrow valleys, and complex urban infrastructure. The integration of 3D LiDAR-derived models enhances spatial resolution and supports microGal-level precision. The proposed compartmentalized terrain correction approach provides a scalable, automated, and accurate alternative to traditional methods, offering substantial benefits for microgravity investigations in rugged terrain and densely built environments.

How to cite: Shahzad, S. and Jadoon, K. Z.: A Compartmentalized Elevation Model Approach to Terrain Correction in Microgravity Surveys, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13520, https://doi.org/10.5194/egusphere-egu26-13520, 2026.

EGU26-15624 | ECS | Orals | EMRP2.2

Airborne Vector Gravimetry Method Based on Independent Gyros Observations 

Wenkai Xiang, Shaokun Cai, Yan Guo, Juliang Cao, Zhiming Xiong, Kaixin Luo, Ruihang Yu, and Meiping Wu

In airborne vector gravimetry algorithms based on SINS/GNSS integrated navigation, the ultimate accuracy of horizontal attitude resolution is primarily constrained by the combined effects of horizontal gravity disturbances and accelerometer measurement errors. Gravity disturbances along the survey line enter the error propagation equations of the strapdown inertial navigation system (SINS) via the sensitivity of accelerometers, forming a closed-loop coupled error propagation chain related to horizontal gravity disturbances. This increases the difficulty of error processing and gravity vector determination. To address this issue, this paper proposes an airborne vector gravimetry method based on independent gyroscopic observation. The method introduces an independent gyros-based attitude determination approach into the traditional SINS/GNSS integrated navigation algorithm. It utilizes the gyroscope assembly of the SINS to independently update the attitude in the inertial frame. The geographic position and time information from GNSS are then used to transform this inertial-frame attitude to the navigation frame for use. A key feature of this method is that it does not employ accelerometer measurements during the attitude update process, thereby avoiding the influence of accelerometer errors and gravity disturbances on the horizontal attitude and achieving decoupling of the closed-loop error propagation chain. Building upon this foundation, the study investigates the linear mapping relationship between the horizontal attitude errors independently resolved by the gyroscope and the horizontal gravity disturbances. Error compensation for airborne gravity vector measurements is performed using gravity anomaly information derived from the EGM2008 model, with both simulated and field data employed for validation. The airborne gravity survey experiments demonstrate that the internal consistency accuracies for the eastward, northward, and upward gravity anomaly components are 1.53 mGal, 2.34 mGal, and 0.59 mGal, respectively, with a spatial resolution of approximately 3 km. This method significantly enhances the decoupling capability between accelerometer measurement errors and gravity disturbances, thereby improving the measurement accuracy of horizontal gravity components.

How to cite: Xiang, W., Cai, S., Guo, Y., Cao, J., Xiong, Z., Luo, K., Yu, R., and Wu, M.: Airborne Vector Gravimetry Method Based on Independent Gyros Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15624, https://doi.org/10.5194/egusphere-egu26-15624, 2026.

EGU26-15998 | ECS | Orals | EMRP2.2

Hex-OSGM: Incremental Gravity Field Learning on Adaptive Hexagonal Meshes for Robust Passive Navigation 

Renjie Zhao, Ruihang Yu, Kaixin Luo, Zhiming Xiong, Juliang Cao, Shaokun Cai, Yan Guo, and Meiping Wu

    Gravity-matching navigation—a self-contained and passive navigation modality—depends critically on the accuracy and resolution of the background gravity field and the adaptability of the matching algorithm,Current gravity modeling methods, however, are limited by slow model updates and inefficient storage under dynamic operating conditions. To overcome these challenges, we introduce a novel gravity-matching framework that integrates incremental learning with adaptive mesh optimization.

    Our approach proceeds in three key stages. First, a global gravity field is rapidly initialized using a spherical-harmonics model trained via an Extreme Learning Machine (ELM). We then employ an online sequential ELM (OS-ELM) to incrementally assimilate posterior gravity information—whether obtained in real time or fused from multi-source observations—thereby enabling timely model updates and continuous refinement of field fidelity.

    Second, we systematically evaluate the sensitivity of batch-matching algorithms (e.g., ICCP and contour matching) to interpolation density and derive an adaptive density-selection criterion that incorporates prior map information content, vehicle velocity, and inertial navigation system error growth. To improve storage and computational efficiency, we replace conventional rectilinear grids with a hexagonal tessellation for field discretization. Theoretical analysis and experimental results confirm that, at equal nominal resolution, the hexagonal lattice reduces both model and localization errors while its structural isotropy enhances the stability and convergence of batch matching across diverse heading angles.

    Third, we introduce an encrypted interpolation strategy centered on hexagonal cell centroids. This approach increases effective resolution with only a minor increase in storage, thereby improving the algorithm’s ability to resolve subtle gravity features. Numerical simulations and field data demonstrate that the proposed framework sustains high-precision matching performance while significantly reducing storage and computational burdens, offering a promising technical pathway toward long-endurance, robust gravity-matching navigation in complex environments.

How to cite: Zhao, R., Yu, R., Luo, K., Xiong, Z., Cao, J., Cai, S., Guo, Y., and Wu, M.: Hex-OSGM: Incremental Gravity Field Learning on Adaptive Hexagonal Meshes for Robust Passive Navigation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15998, https://doi.org/10.5194/egusphere-egu26-15998, 2026.

EGU26-18750 | ECS | Posters on site | EMRP2.2

An Inversion Method for Moho Depth Distribution Characteristics in the Bohai Sea and Its Adjacent Areas Based on the Improved Bott-Parker Method 

Guanghong Lan, Juliang Cao, Zhiming Xiong, Kaixin Luo, Ruihang Yu, Shaokun Cai, Yan Guo, and Meiping Wu

Abstract. The Bohai Sea and its adjacent areas (116.5°~123.5°E, 36.5°~41.5°N) are located in eastern China, serving as a critical marine-continental transition zone in the eastern part of the country. Acquiring high-precision distribution characteristics of the Moho depth in this region is of great significance for understanding the local deep tectonic features and the distribution of mineral resources such as oil and gas. Owing to the high cost of seismic surveys, it is difficult to obtain the overall Moho topography of the region. Therefore, based on the latest generation of SWOT-03 satellite gravity data, this study uses the improved Bott-Parker method to invert a high-resolution Moho topography with a resolution of 1′×1′ in the Bohai Sea and its adjacent areas. First, Bouguer correction was applied to the SWOT-03 free-air gravity anomalies to derive the Bouguer gravity anomalies of the study area. To separate the Moho gravity anomalies, which reflect the distribution characteristics of the Moho depth, from the Bouguer gravity anomalies, an 8th-order wavelet multiscale decomposition was performed on the Bouguer gravity anomalies, generating the corresponding wavelet approximations and wavelet details. Then, the average radial logarithmic power spectrum analysis method was used to calculate the approximate source depths of the wavelet details of each order, thus obtaining the gravity anomalies that represent Moho undulation. Finally, the improved Bott-Parker method was employed to invert the high-resolution Moho topography of the Bohai Sea and its adjacent areas. Specifically, the improved Bott-Parker method obtains the initial Moho topography via linear regression using known seismic Moho data and Moho gravity anomalies derived from wavelet multiscale decomposition, and then continuously corrects the Moho topography using the gravity difference between the forward-calculated values from the Parker method and the observed gravity values. Compared with the traditional Parker-Oldenburg method, the improved Bott-Parker method avoids the need to set the cutoff frequency of the filter. The results demonstrate that the average Moho depth in the Bohai Sea and its adjacent areas is 32.98 km, with a variation range of 24.26~57.22 km, and multiple Moho uplift and depression zones are present in the region. The inverted Moho topography is basically consistent with the Crust1.0 global crustal model, which can well reflect the distribution characteristics of the Moho depth in the Bohai Sea and its adjacent areas as a whole. This study has certain guiding significance for understanding the regional tectonic features and conducting oil and gas exploration.

Keywords: SWOT-03 satellite gravity data; Moho depth; Gravity inversion; Wavelet multi-scale decomposition;Improved Bott-Parker method

How to cite: Lan, G., Cao, J., Xiong, Z., Luo, K., Yu, R., Cai, S., Guo, Y., and Wu, M.: An Inversion Method for Moho Depth Distribution Characteristics in the Bohai Sea and Its Adjacent Areas Based on the Improved Bott-Parker Method, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18750, https://doi.org/10.5194/egusphere-egu26-18750, 2026.

EGU26-19348 | Posters on site | EMRP2.2

Aeromagnetic Mapping in the Northern Tihamah region, Western Yemen 

Marwan Al-Badani and Fausto Ferraccioli

The basement geology of Yemen is related to the evolution of the late Archean to late Neoproterozoic Arabian-Nubian Shield and contains key records of microplate and island arc accretion during Gondwana assembly. Furthermore, Yemen also preserves important igneous and structural records related to the multi-stage extension and opening of the Gulf of Aden-Red Sea Rift System.

Here we focus on the interpretation of aeromagnetic anomaly data in western Yemen by analysing part of a magnetic anomaly compilation for the whole of Yemen that includes data collected from 26 different airborne surveys flown between 1976 and 1985.

Our reduced to the pole map reveals magnetic anomalies of varying amplitudes and wavelengths, reflecting differences in lithology, structure, and source depth. We applied edge-detection techniques, including tilt angle derivative, total horizontal derivative of the tilt angle, and 3D Euler deconvolution to aid depth to source estimation.

An intriguing result is the newly defined extent of largely buried Cenozoic igneous intrusions that we image from the scant exposures along the southern uplifted rift-related great escarpment to the downthrown block in the northern Tihamah plain. The trend of these anomalies lies at relatively high angle to the rift flank escarpment but is co-linear with some of the trends imaged in the Precambrian basement, suggesting an important role of the inherited structures on much later magma emplacement. To further contextualise our regional results we combine the data from western Yemen with lower resolution publically available data from adjacent sectors of the Arabian shield and the Red Sea Rift and discuss some of the potential tectonic implications.

How to cite: Al-Badani, M. and Ferraccioli, F.: Aeromagnetic Mapping in the Northern Tihamah region, Western Yemen, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19348, https://doi.org/10.5194/egusphere-egu26-19348, 2026.

EGU26-19968 | Posters on site | EMRP2.2

A Multi-Method Gravity Workflow for Reliable Structural Mapping in Northern Tunisia 

imen hamdi, Mohamed Sobh, Adnen Amiri, and inoubli Mohamed hédi

High-resolution gravity data were used to assess their potential and limitations as a subsurface investigation tool to constrain key geological structures and support georesource exploration in Northwestern Tunisia. In this structurally complex area, methodological choices—particularly those related to regional–residual separation, derivative filtering, interpolation schemes, and Euler-based depth-estimation parameters—significantly influence the geometry, continuity, and uncertainty of interpreted lineaments.

To mitigate these effects, we applied an integrated multi-stage workflow combining residual anomaly mapping, derivative filters, tilt-angle transformation, power-spectrum analysis, Euler deconvolution of horizontal gradients (EHD), and 3D Euler solutions. These complementary approaches delineate subsurface fault systems and highlight deep structural controls on Triassic salt diapirs and associated Pb–Zn mineralization. The results reveal a dominant NE–SW structural corridor with fault depths reaching ~1.75 km, spatially correlating with known mineralized sites and salt-dome boundaries.

To further enhance structural reliability and quantify subsurface density distributions, the workflow incorporates 3D gravity inversion. The inversion model helps image density contrasts associated with the Triassic evaporites, validating interpreted lineaments and refining depth estimates derived from derivative-based and Euler approaches. Integrating forward–inverse modelling with classical interpretation tools not only enhances the structural understanding but also provides a clear workflow, helping users assess the reliability and limitations of gravity-derived structural maps in tectonic complex areas.

 

How to cite: hamdi, I., Sobh, M., Amiri, A., and Mohamed hédi, I.: A Multi-Method Gravity Workflow for Reliable Structural Mapping in Northern Tunisia, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19968, https://doi.org/10.5194/egusphere-egu26-19968, 2026.

EGU26-21409 | Orals | EMRP2.2

Enhanced magnetic and gravity imaging of the crustal basement beneath the northern Wilkes Subglacial Basin in East Antarctica 

Fausto Ferraccioli, Shi Quan Ooi, Marwan A. Al-Badani, Duncan Young, Donald Blankenship, Egidio Armadillo, Joerg Ebbing, and Martin Siegert

The Wilkes Subglacial Basin (WSB) is one of the largest tectonic features in East Antarctica as it stretches for almost 1600 km from the Southern Ocean towards South Pole. Significant research has focussed on the tectonic origin of the basin with competing models ranging from Paleozoic, Mesozoic and Cenozoic extensional models to flexural models related to the Cenozoic uplift of the Transantarctic Mountains. Comparatively little effort has however been placed on investigating the cryptic basement of the WSB despite its key location at the transition between the exposures of the Archean-Mesoproterozoic Terre Adelie Craton and the late Neoproterozoic to Ordovician age Ross Orogen.

Here we present enhanced aeromagnetic and airborne gravity imaging augmented by satellite magnetic and satellite gravity data and comparisons with formerly adjacent southeastern Australia to redefine key features of the basement in the northern WSB region.

We show that a prominent magnetic low located beneath the Western Basins within the WSB is not caused by a ca 3 km thick Cambrian rift basin as previously proposed (Ferraccioli et al., 2009, Tectonophysics) but images instead a linear Archean crustal ribbon extending further north to exposures of Archean rocks in the Terre Adelie craton and in the Gawler Craton. Cambrian sedimentary basins are confirmed further east beneath the northern Central Basins. Prominent magnetic highs along the eastern flank of the WSB and at the edge of the southern Central Basins were previously interpreted to reveal Ross age igneous basement associated with an arc-back arc system. However, the occurrence of longer wavelength satellite magnetic anomalies both in the WSB and at the edge of the Gawler Craton and in the Curnamona Craton in Australia lead us to propose an alternative hypothesis that predicts the occurrence of more extensive Paleo to Mesoproterozoic basement than previously inferred. Furthermore, a prominent linear residual gravity anomaly along the western flank of the WSB is interpreted here as reflecting uplifted mafic lower crust associated with Paleoproterozoic rifting. High amplitude aeromagnetic anomalies may reflect coeval banded iron formations associated at shallower crustal levels with such Paleoproterozoic rifting processes.

By comparing gravity signatures over the WSB and southern Australia and by incorporating recent seismic constraints at the transition between the Gawler Craton and the Delamerian Orogen we reassess the extent and architecture of both the Precambrian and Cambrian basement.

Overall, our results and models have significant implications for tectonic studies of the basement of the WSB, including better defining the role of inherited tectonics structures on the more recent  Paleozoic, Mesozoic to Cenozoic evolution of the WSB. Furthermore, the larger degree of heterogeneity in the crustal basement identified here will help inform next generation models of intracrustal contributions to geothermal heat flow  beneath this key sector of the East Antarctic Ice Sheet.

How to cite: Ferraccioli, F., Ooi, S. Q., Al-Badani, M. A., Young, D., Blankenship, D., Armadillo, E., Ebbing, J., and Siegert, M.: Enhanced magnetic and gravity imaging of the crustal basement beneath the northern Wilkes Subglacial Basin in East Antarctica, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21409, https://doi.org/10.5194/egusphere-egu26-21409, 2026.

EGU26-21850 | Posters on site | EMRP2.2

Quantitative Assessment of CO2 Leakage Using Time-Lapse Gravity Inversion 

Maurizio Milano, Alessia Ianniello, Marco Maiolino, Luigi Bianco, and Maurizio Fedi

We propose an innovative approach for the interpretation of time-lapse gravity data aimed at estimating subsurface mass variations associated with CO2 injection and storage. The method is based on the Extremely Compact Source (ECS) inversion technique (Maiolino et al., 2024), which is used to isolate the individual contributions of discrete CO2 mass accumulations in the subsurface and to quantify their associated excess mass.

To date, ECS inversion has been primarily applied as a filtering strategy to remove regional-scale contributions from potential field data or to separate the effects of closely spaced sources. The approach relies on an iterative inversion of potential field observations to derive a subsurface model composed of source distributions with minimal volumetric extent, referred to as atoms, simultaneously ensuring a low data misfit. A key advantage of the method is that it does not require any a priori information about subsurface properties.

Once the ECS model is obtained, the excess mass associated with each source contributing to the observed gravity anomaly can be readily computed. In this study, we demonstrate that the proposed approach enables precise identification of CO2 accumulations within the reservoir and allows for accurate estimation of net mass variations related to both stored CO2 and leakage occurring along permeable fault zones.

 

How to cite: Milano, M., Ianniello, A., Maiolino, M., Bianco, L., and Fedi, M.: Quantitative Assessment of CO2 Leakage Using Time-Lapse Gravity Inversion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21850, https://doi.org/10.5194/egusphere-egu26-21850, 2026.

GI6 – Multidisciplinary Sensor Networks for Environmental Applications

Wetlands are unique ecological systems that exhibit both aquatic and terrestrial landscape characteristics. Wetland water quality is facing significant threats due to the combined impacts of climate variations and human activities. Therefore, analyzing the spatiotemporal dynamics of water clarity (Secchi disk depth, Zsd) across different types of wetlands, as well as revealing the relationship between driving factors and their responses, is crucial for monitoring and assessing variations in wetland water environments. The study utilizes Landsat data to analyze the spatiotemporal dynamics of Zsd and the response relationships of driving factors in typical flow-connected and non-flow-connected lake wetlands since 1984, focusing on Dongting Lake (DTL) and Poyang Lake (PYL) as examples of river-flow lake wetlands, and Baiyangdian Lake (BYD) and Hengshui Lake (HSL) as examples of non-flow-connected lake wetlands. The findings reveal that the variations in Zsd and the spatial variability in river-flow connected lake wetlands are greater than those in non-flow-connected lake wetlands, which may be attributed to abundant precipitation and frequent water exchanges. In terms of interannual scale, distinct stages of increase and decrease in Zsd are observed, characterized by peak values followed by declines. These interannual variations are driven not only by climate fluctuations but also by variations in landuse and landscape. Through quantitative analysis of the spatiotemporal dynamics of Zsd in various wetland types, the study further explores the driving mechanisms and the differing responses of climate factors, landuse, and landscape to Zsd variations in river-flow and non-flow-connected lake wetlands. The research provides a data foundation and scientific support for monitoring and managing water resources in large-scale wetlands under the dual impacts of climate variability and human activities.

How to cite: Zhao, Y.: Contrasting Drivers of Water Clarity: A Multi-Decadal Satellite Analysis of Two Types of Lake Wetlands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-61, https://doi.org/10.5194/egusphere-egu26-61, 2026.

EGU26-1312 | ECS | Orals | GI6.1

Predictive analysis of Urban Heat Islands using satellite data and neural network algorithms  

Lucia Cavallaro, Michele Mangiameli, and Giuseppe Mussumeci

The Urban Heat Island (UHI) phenomenon is a critical concern, particularly in the context of global warming and rapid urbanization. UHIs are essentially urbanized areas that exhibit higher temperatures compared to their less or non-urbanized surroundings. This heat island effect is worsened by urbanization, largely due to the extensive use of asphalt and other impervious surfaces over green spaces, coupled with various human activities. The environmental conditions created by UHIs negatively impact the quality of life. These areas suffer from elevated temperatures, higher concentrations of pollutants, and a subsequent increase in the energy and economic costs associated with cooling buildings. Numerous studies have been carried out to tackle the growing issue of the UHI. These efforts concentrate on analyzing UHI features to equip environmental planners and decision-makers with vital instruments for mitigation and management. This work investigates the UHI phenomenon in the Catania area (Sicily, Italy), focusing on a specific urban section to highlight the contrast between densely built and greener spaces. The study employs remote sensing data from Landsat 8 and 9 satellite missions to calculate relevant indices, such as the Normalized Difference Vegetation Index (NDVI) and Land Surface Temperature (LST), which are essential for UHI analysis. After generating a thematic map of UHIs for the area, the Land Use Land Cover (LULC) was analyzed. This LULC analysis facilitated the use of the QGIS MOLUSCE plug-in, a tool offering several algorithms for predictive LULC modeling. The available algorithms include neural networks (multilayer perceptron), logistic regression, weights of evidence, multi-criteria evaluation, and validation via kappa statistics. The model's results were validated by projecting them onto a year for which actual data was already available. Predictive LULC modeling enables the evaluation of UHI conditions at the time of the projection. This capability makes the tool valuable for environmental planners and decision-makers, aiding in the assessment of future urbanization impacts and their subsequent effects on the population's quality of life. 

How to cite: Cavallaro, L., Mangiameli, M., and Mussumeci, G.: Predictive analysis of Urban Heat Islands using satellite data and neural network algorithms , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1312, https://doi.org/10.5194/egusphere-egu26-1312, 2026.

EGU26-3533 | ECS | Posters on site | GI6.1

Data-driven environmental monitoring of soil potentially toxic elements using multisource remote sensing and Machine Learning 

Maria Silvia Binetti, Carmine Massarelli, Jonathan Vidal Solórzano Villegas, Jean Francois Mas, Emanuele Barca, and Vito Felice Uricchio

Soil contamination monitoring in industrialized regions requires accurate, spatially continuous assessments. We present an integrated remote sensing framework for predicting concentration of soil Potentially Toxic Elements (Cd, Be, V, Cr, As, Co), which were selected based on their significant correlations with hyperspectral and multispectral signatures observed in preliminary exploratory chemical analysis. The framework integrates PRISMA hyperspectral, Sentinel-2 multispectral, and DEM-derived topographic data, tested near the industrial area of Taranto (southern Italy), a priority site for environmental risk assessment.

Our methodology integrates heterogeneous satellite data through systematic preprocessing, spectral index computation, morphometric feature extraction, and spatially feature selection. A correlation-based selection algorithm with a spectral distance constraint (∆λ<30 nm) was specifically implemented to mitigate multicollinearity inherent in high-dimensional hyperspectral data, ensuring the selection of non-redundant predictors. Machine learning regression models were trained on laboratory measured soil samples and validated via stratified cross-validation and independent holdout data.

Results demonstrate differential model performance across PTEs: R² = 0.75–0.82 (training) and 0.58–0.68 (validation). Feature importance analysis revealed complementary contributions from hyperspectral bands, multispectral indices, and terrain morphology, with hyperspectral data providing the strongest discriminative power. Single-sensor approaches (Sentinel-2 only) yielded notably lower performance, confirming the value of data integration. High-resolution maps identified the most polluted areas, validating the framework's capability for spatial assessment of soil contamination hotspots.

How to cite: Binetti, M. S., Massarelli, C., Solórzano Villegas, J. V., Mas, J. F., Barca, E., and Uricchio, V. F.: Data-driven environmental monitoring of soil potentially toxic elements using multisource remote sensing and Machine Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3533, https://doi.org/10.5194/egusphere-egu26-3533, 2026.

EGU26-6614 | ECS | Orals | GI6.1

A GIS-enabled spectral library to disseminate field data for surface spectroscopy 

Marco Solinas, Massimo Musacchio, Malvina Silvestri, Maria Fabrizia Buongiorno, Sergio Falcone, Maria Teresa Melis, Marco Casu, and Salvatore Noli

Remote sensing from ground, UAV, aircraft and satellite platforms is increasingly central to monitoring Earth’s surface and supporting decision making. However, robust interpretation of multispectral/hyperspectral observations still depends on consistent links between satellite products and high-quality reference spectra measured in the field and laboratory, plus workflows that make these data interoperable across sensors, spatial scales and acquisition conditions. We present the INGV Spectral Library, a web-based, GIS-integrated platform designed to operationally connect in situ spectroscopy with airborne/satellite imaging spectroscopy, enabling reproducible pre-processing, cross-sensor harmonization, and geospatial querying of spectral datasets for environmental monitoring applications.

The platform provides standardized spectral analytics commonly required in monitoring pipelines: continuum removal and absorption-feature characterization, derivative-based enhancement to emphasize diagnostic features, and sensor-aware resampling using Spectral Response Functions (SRFs) to harmonize high-resolution field spectra to specific sensors (e.g., Sentinel-2 and spaceborne hyperspectral missions). This “sensor-to-field” alignment enables direct comparability and supports spectral–spatial data fusion, where field-based endmembers and satellite reflectance/emissivity products can be jointly analysed. A key component is the GIS interface: spectra are linked to georeferenced samples and metadata and can be filtered by location, lithology/land cover context, acquisition conditions and spectral criteria, facilitating rapid exploration of spatial patterns and targeted selection of reference signatures for mapping and validation tasks.

Two use cases illustrate the relevance to environmental monitoring and hazard-related contexts. (i) In Sardinia (Sale ’e Porcus), curated VNIR–SWIR FieldSpec measurements are ingested as a controlled reference set to support multi-sensor consistency checks and calibration/validation activities for satellite imaging spectroscopy. (ii) In Oman, PRISMA Level-2D surface reflectance is analysed through spectral indices and Spectral Angle Mapper (SAM), using PRISMA-resampled endmembers derived from reference spectra to delineate spatially coherent alteration patterns and potential copper-related signals; the resulting maps support field planning and prioritization of sampling targets, with new samples intended to validate and refine satellite-based interpretations.

By combining standardized spectral pre-processing, SRF-based cross-sensor harmonization, and GIS-driven access to reference spectra, the INGV Spectral Library provides a practical platform for multi-scale environmental remote sensing, enabling more transparent, transferable and decision-oriented workflows for monitoring surface changes and hazard-relevant processes.

This study is carried out within two projects: the Space It Up project funded by the Italian Space Agency, ASI, and the Ministry of University and Research, MUR, under contract n. 2024-5-E.0 - CUP n. I53D24000060005 and  PRIN2022_SH6_2022BTKA9Y-02 funded by  Ministry of University and Research, MUR CUP  D53D23000580006.

How to cite: Solinas, M., Musacchio, M., Silvestri, M., Buongiorno, M. F., Falcone, S., Melis, M. T., Casu, M., and Noli, S.: A GIS-enabled spectral library to disseminate field data for surface spectroscopy, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-6614, https://doi.org/10.5194/egusphere-egu26-6614, 2026.

EGU26-7030 | ECS | Posters on site | GI6.1

High-resolution multi-sensor UAS framework for individual tree health monitoring and structural analysis in walnut orchards 

Issa Loghmanieh, Amjad Hamdan, Géza Bujdosó, Kourosh Vahdati, and László Bertalan

Persian or English Walnut (Juglans regia L.) growing in Hungary faces significant challenges from complex biotic pathogens and abiotic climate stressors. While farmers possess the expertise to identify these pathologies, early diagnosis is often impeded by the physical inaccessibility of the upper canopy, where symptoms frequently manifest first. To overcome these limitations, this study proposes a multi-sensor Unmanned Aerial System (UAS) framework capable of acquiring high-resolution geospatial data to identify physiological features invisible to the human eye.

The research was conducted at two distinct sites in Central Hungary, representing contrasting management regimes. The first is a 2.4-hectare intensive commercial orchard utilizing rigorous irrigation and chemical protection. The second is a 4.2-hectare genetic archive owned by the HUALS Fruit Growing Research Center; this site contains diverse cultivars with varying management levels (including untreated controls), offering a higher probability of observing heterogeneous disease responses.

Data acquisition utilized a DJI Matrice M210 equipped with a 10-band MicaSense RedEdge-MX Dual system and a DJI Matrice M350 RTK with a Zenmuse L2 LiDAR sensor. To assess the impact of spatial resolution on disease identification accuracy, multispectral surveys were conducted at altitudes of 40, 57, and 72 m AGL, resulting in GSDs of 3, 4, and 5 cm/pixel, respectively. Surveys were conducted in June 2025 to establish baseline pre-symptomatic conditions and repeated in September 2025 during the pre-harvest period, when symptoms were clearly visible. LiDAR data was collected once to characterize stable structural parameters, such as tree height and crown complexity.

For tree-level analysis, precise individual tree crown delineation is essential. While point cloud-based segmentation was evaluated, a more robust delineation was achieved by integrating Deep Learning algorithms applied to RGB orthophotos. The 10-band spectral data facilitated the calculation of sensitive narrow-band indices (e.g., PRI, NDRE, Cl_RE) to detect changes in pigmentation and photosynthetic efficiency. Finally, the study applies multivariate statistical analysis to cluster trees by fusing 3D structural metrics derived from LiDAR with spectral indices. This approach aims to model species-specific stress responses and categorize cultivars based on their physiological and structural characteristics, providing a foundation for improved precision agriculture workflows.

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Issa Loghmanieh is funded by the Stipendium Hungaricum scholarship under the joint executive program between Hungary and Iran.

How to cite: Loghmanieh, I., Hamdan, A., Bujdosó, G., Vahdati, K., and Bertalan, L.: High-resolution multi-sensor UAS framework for individual tree health monitoring and structural analysis in walnut orchards, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7030, https://doi.org/10.5194/egusphere-egu26-7030, 2026.

EGU26-7537 | ECS | Orals | GI6.1

Multi-Temporal Road Surface Classification from Sentinel-2 and OpenStreetMap Data Using Deep Learning 

Magdalena Halbgewachs, Marc Wieland, Anne Schneibel, Christian Geiß, and Monika Gähler

During natural hazards and other rapidly evolving crisis situations, the accessibility of evacuation routes and the delivery of emergency supplies strongly depends on road surface type. However, in many regions affected by environmental changes, conflicts, or population displacement, reliable information on road surface conditions is incomplete, outdated, or entirely unavailable, which limits effective disaster response and environmental monitoring. This study presents a satellite-based framework that classifies roads as either paved or unpaved using multispectral Sentinel-2 imagery and volunteered geographic information (VGI) from OpenStreetMap (OSM).
OSM road geometries are used to extract spectral samples from Sentinel-2 surface reflectance data, which is used to train a convolutional neural network (CNN) for road surface classification across diverse environmental settings. To improve spatial consistency and practical usability, classification results are aggregated at the road-segment level to produce coherent surface classifications aligned with real-world road infrastructure. The framework is designed to be transferable and applicable across regions with varying climates, land-cover characteristics, and degrees of urbanisation.
The approach has been evaluated across multiple target regions and demonstrates consistent performance beyond the training domain, which highlights its potential for cross-regional application. Due to the regular revisit time of Sentinel-2, the framework further supports multi-temporal analysis. This makes it possible to assess changes to the road surface before and after dynamic events, such as flood-induced degradation, sediment coverage or long-term urbanization.  By combining freely available satellite data and open VGI, the proposed method provides a scalable tool for infrastructure monitoring, disaster response, and environmental assessment in data-scarce and rapidly changing regions.

How to cite: Halbgewachs, M., Wieland, M., Schneibel, A., Geiß, C., and Gähler, M.: Multi-Temporal Road Surface Classification from Sentinel-2 and OpenStreetMap Data Using Deep Learning, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7537, https://doi.org/10.5194/egusphere-egu26-7537, 2026.

EGU26-7807 | ECS | Orals | GI6.1

Towards reliable X-band InSAR monitoring of complex deformation: Insights from the 2024-2025 Fentale-Dofen Magma Intrusion 

Weiyu Zheng, Juliet Biggs, Lin Way, Milan Lazecky, and Raphael Grandin

Recent advances in satellite remote sensing, particularly high-resolution and high-temporal-frequency SAR systems, provide new opportunities for capturing rapidly evolving deformation. X-band InSAR (Interferometric Synthetic Aperture Radar) data from the COSMO-SkyMed (CSK) and COSMO-SkyMed Second Generation (CSG) constellations offer dense temporal sampling and high spatial resolution, making them particularly valuable for monitoring complex, rapidly evolving deformation signals. However, the short wavelength of X-band data can make phase unwrapping – the step required to convert wrapped interferometric phase into continuous surface displacement – challenging when the signal has a large footprint, large deformation gradients and surface discontinuities.

Here we present an enhanced X-band InSAR monitoring framework applied to the 2024-2025 Fentale-Dofen dyke intrusion in Ethiopia. The dyke measured ~50 km in length and produced complex surface deformation spanning ~10,500 km², with InSAR line-of-sight displacements up to ~3 m over ~60 days. Monitoring dyke intrusion-related deformation is important for understanding magma movement, assessing volcanic hazards, and supporting rapid response during period of unrest. We address limitations of conventional phase unwrapping in areas of complex deformation, including dense fringes caused by dyke-opening and discontinuous deformation within the graben. By integrating pixel-offset tracking with interferometric phase, we develop a reliable offset-supported unwrapping strategy that allows robust recovery of surface displacement associated with both dyke opening and graben subsidence, with consistency evaluated by loop-closure tests. The resulting deformation products provide a consistent basis for InSAR time-series analysis using dense CSK observations, allowing the temporal evolution of intrusion-related deformation to be resolved at high spatial and temporal resolution. Ongoing work extends this framework toward integrated deformation modeling, combining geodetic observations with physics-based representations of dyke-driven magma transport to better constrain subsurface processes.

This study demonstrates how advanced InSAR processing strategies and multi-technique data integration can unlock the full potential of high-resolution X-band SAR data for environmental hazard monitoring. The proposed framework contributes to the development of robust remote sensing tools for deformation analysis, supporting both near-real-time monitoring and post-event assessment of volcanic and other hazards.

How to cite: Zheng, W., Biggs, J., Way, L., Lazecky, M., and Grandin, R.: Towards reliable X-band InSAR monitoring of complex deformation: Insights from the 2024-2025 Fentale-Dofen Magma Intrusion, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7807, https://doi.org/10.5194/egusphere-egu26-7807, 2026.

EGU26-9147 | Posters on site | GI6.1

Spatial stratification method for the sampling design of remote sensing classification accuracy assessment 

Shiwei Dong, Yu Liu, Yunbing Gao, and Yanbing Zhou

Spatial sampling design is essential for accurately assessing land use and land cover (LULC) classification results from remote sensing data. When classification correctness exhibits spatial heterogeneity, spatial stratification can significantly improve spatial sampling efficiency by dividing the study area into heterogeneous strata. Three spatial stratification methods were introduced, respectively focusing on LULC types, the integration of multi-source classification products with different spatial resolutions, and pixel-level uncertainty analysis.

First, stratification by LULC types was employed because these categories directly relate to variations in classification accuracy. Second, although LULC products from different sources and resolutions were generated using diverse data and methods, their consistency and inconsistency could indicate potential misclassification. Thus, a stratification method that combined such multi-source products was developed for guiding accuracy assessment sampling. Third, a pixel-based stratification framework was proposed based on uncertainty indices, namely the maximum probability, fuzzy confusion index, and probability entropy.

The effectiveness of these methods was tested through a case study of LULC classification in Beijing, China. Results showed that the proposed stratification approaches could effectively distinguish spatial characteristics and improve sample representativeness, thereby optimizing the sampling for classification accuracy evaluation and enhancing its overall reliability.

How to cite: Dong, S., Liu, Y., Gao, Y., and Zhou, Y.: Spatial stratification method for the sampling design of remote sensing classification accuracy assessment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9147, https://doi.org/10.5194/egusphere-egu26-9147, 2026.

EGU26-10170 | Posters on site | GI6.1

Advancements in volcanological Earth observation: Documenting the February 2025 eruption of Mount Etna 

Annalisa Cappello, Gaetana Ganci, Giuseppe Bilotta, Maddalena Dozzo, Francesco Spina, Francesco Zuccarello, Roberta Cristofaro, and Marco Spina

Earth Observation data has become an increasingly indispensable resource in the field of volcanology, providing unprecedented capabilities for the high-resolution assessment of the timing, magnitude, and explosivity of active eruptive events. This work leverages a multi-sensor suite of satellite-derived products to meticulously document the February 2025 eruption of Mount Etna, Italy. This specific event holds particular significance as it represents the first major eruption fully monitored with the operational third-generation Meteosat satellite (Meteosat Third Generation - Imager, MTG-I), which offers a revolutionary advancement in mid-infrared spatial and temporal resolution for thermal monitoring. 

Daily SkySat/PlanetScope imagery monitored effusive activity and lava flow dynamics, providing high-cadence data on flow evolution and areal expansion, yielding critical insights into flow propagation rates and the spatial distribution of the effusive material. Magma supply rates and thermal output were assessed by tracking eruption-related thermal anomalies using multi-sensor data (MODIS, SEVIRI, VIIRS, FCI aboard MTG-I), enabling the calculation of the volume of extruded magma per unit time. Eruptive plumes and volcanic gas monitoring, including TROPOMI SO₂ total mass estimates, analyzed the explosive component and atmospheric impact of the eruption. Finally, high-resolution Pléiades imagery acquired rapidly post-eruption allowed for generating an updated Digital Surface Model (DSM). DSM differencing with a pre-eruptive reference precisely estimated deposit thickness and total erupted volume.

This interdisciplinary work provides essential information for analyzing multi-temporal morphological changes and conducting comprehensive hazard assessment studies, thereby contributing significantly to efforts aimed at mitigating the impact of environmental hazards.

This research has been supported by the INGV project Pianeta Dinamico VT SAFARI — CUP D53J19000170001— funded by Italian Ministry MIUR (“Fondo Finalizzato al rilancio degli investimenti delle amministrazioni centrali dello Stato e allo sviluppo del Paese”, legge 145/2018) and by the Space It Up project — CUP I53D24000060005 — funded by the Italian Space Agency and the Ministry of University and Research, under contract n. 2024-5-E.0.

How to cite: Cappello, A., Ganci, G., Bilotta, G., Dozzo, M., Spina, F., Zuccarello, F., Cristofaro, R., and Spina, M.: Advancements in volcanological Earth observation: Documenting the February 2025 eruption of Mount Etna, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10170, https://doi.org/10.5194/egusphere-egu26-10170, 2026.

EGU26-10620 | ECS | Orals | GI6.1

Effect of Spatial Resolution on Land Cover Mapping in an Agropastoral Area of Niger (Aguie and Mayahi) Using Sentinel-2 and Landsat 8 Imagery within a Random Forest Regression Framework 

Sanoussi Abdou Amadou, Dambo Lawali, Jean-François Bastin, Jan Bogaert, Adrien Michez, and Jeroen Meersmans

Monitoring environmental changes over time requires image time series with extensive historical depth. However, high spatial resolution images often lack such depth. Additionally, some remote areas may suffer from either insufficient satellite coverage or a lack of high-resolution or high-quality imagery.  This study aims to investigate the impact of spatial resolution on image classification. Therefore, Landsat 8 and Sentinel-2 images from October to December 2020 were processed and classified using Random Forest regression in Google Earth Engine (GEE).  Training samples were collected from Collect Earth Online (CEO) to train the model. In addition to the spectral bands available, vegetation indices were considered to optimize classification results. The study revealed differences in land cover areas estimated by the two sensors. These differences are statistically significant at p < 0.001, although they are small. The validation results showed that the RMSE from Sentinel-2 is slightly lower than that from Landsat 8. Although small, this difference is significant at p < 0.05. This highlights two key points: (i) that spatial resolution positively influences the accuracy of image classification, especially when dealing with Landsat 8 and Sentinel-2 imagery; and (ii) that the difference between Landsat 8 and Sentinel-2 sensors is not too substantial in the context of a fragmented landscape, since it ranged from 0.03% to 3.94% across land covers. Therefore, Landsat imagery and, by extension, medium-resolution satellite imagery can still yield satisfactory land cover maps, especially in a patchy landscape such as the southeastern part of Niger.

Keywords: Stratified random sampling; Google Earth Engine (GEE); Random Forest; Collect Earth Online (CEO); Niger

How to cite: Abdou Amadou, S., Lawali, D., Bastin, J.-F., Bogaert, J., Michez, A., and Meersmans, J.: Effect of Spatial Resolution on Land Cover Mapping in an Agropastoral Area of Niger (Aguie and Mayahi) Using Sentinel-2 and Landsat 8 Imagery within a Random Forest Regression Framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10620, https://doi.org/10.5194/egusphere-egu26-10620, 2026.

EGU26-12633 | Posters on site | GI6.1

Monitoring Long-term Vegetation Phenology across Europe Using Satellite NDVI Time Series (PKU GIMMS) 

Caterina Samela, Vito Imbrenda, Rosa Coluzzi, and Maria Lanfredi

Large-scale and long-term satellite observations are essential for environmental monitoring and for detecting gradual ecosystem responses to climate variability and land-use change.

This study presents a remote sensing–based framework to characterize vegetation phenology and its stability across Europe over four decades (1982–2022), using the temporally consistent and cross-sensor-calibrated PKU GIMMS NDVI dataset. The framework integrates NDVI time-series analysis with a newly developed Phenology Variability Index (PVI), designed to assess phenological stability at climatic scales and to complement established methods. Monthly NDVI time series are analyzed using non-parametric statistical tests and long-term mean seasonal profiles to delineate phenologically coherent regions through spatial clustering. Land Surface Phenology (LSP) metrics and the Phenology Variability Index are subsequently derived to characterize seasonal timing, trends, and phenological stability within and across regions. In this way, we integrate spatially explicit, pixel-level NDVI statistics and PVI-based evaluations with analyses of phenologically homogeneous clusters, providing a comprehensive understanding of vegetation dynamics across ecosystems.

Five spatially coherent clusters were identified, each characterized by distinct seasonal signatures linked to major European eco-climatic zones. Results reveal pronounced spatial and temporal heterogeneity, with consistent greening trends in temperate, montane, and Mediterranean regions, weaker and seasonally constrained greening in semi-arid areas, and largely stable winter NDVI conditions in mountainous forests and continental regions. LSP metrics indicate shifts in the timing and duration of the growing season, reflecting combined effects of climate variability and land-use change. The PVI further highlights higher phenological stability in Mediterranean and semi-arid landscapes, contrasted with greater variability in temperate and montane ecosystems.

Overall, this study demonstrates how long-term, high-temporal-resolution satellite data can support ecosystem assessment and environmental monitoring across continental scales. The proposed framework provides a transferable and robust methodological basis for analyzing vegetation dynamics, contributing to remote sensing–driven environmental monitoring and climate change research.

 

Keywords:
Remote sensing; Environmental monitoring; Vegetation dynamics; NDVI time series; Europe; Phenology Variability Index (PVI); Monthly trend analysis; Land Surface Phenology.

How to cite: Samela, C., Imbrenda, V., Coluzzi, R., and Lanfredi, M.: Monitoring Long-term Vegetation Phenology across Europe Using Satellite NDVI Time Series (PKU GIMMS), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12633, https://doi.org/10.5194/egusphere-egu26-12633, 2026.

EGU26-12873 | Posters on site | GI6.1

GPP from two decades of MSG data for terrestrial ecosystem monitoring over Europe and Africa 

Beatriz Martinez, M. Amparo Gilabert, Sergio Sánchez-Ruiz, Manuel Campos-Taberner, Adrián Jiménez-Guisado, and F. Javier García-Haro

One of the main carbon fluxes characterizing terrestrial ecosystems and biodiversity is gross primary production (GPP), defined as the amount of carbon fixed by vegetation through photosynthesis, per unit area and unit time. GPP represents the potential carbon uptake of an ecosystem to produce food, wood, and fiber. Therefore, understanding its spatiotemporal variability under future climate change scenarios is essential for environmental management and global sustainable development. The temporal variability can be characterized by analyzing GPP time series, which exhibit non-stationary behavior driven by short-term, seasonal, and long-term variations.

In the last decade, significant advancements have been achieved in the development and production of operational long-term GPP series using Earth Observation (EO)-based data at regional and global scale. This is the case of the 10-day GPP product at 3.1 km (MGPP LSA-411) from geostationary SEVIRI/MSG data within the LSA SAF (Land Surface Analysis SAF) as part of the SAF (Satellite Application Facility) network of EUMETSAT. This product is freely available in the LSA SAF platform since 2018 for addressing near-real-time users’ climate and environmental applications. Currently, the possibility of improving this product using a new version of fAPAR, now under development, is being analyzed. This work aims to provide a 20-year assessment (2004–2023) of terrestrial ecosystem status based on the spatiotemporal analysis of 10-day GPP time series derived from MSG data, following the methodology of the operational MGPP product (LSA-411) but using a novel fAPAR as input based on a deep-learning approach.

In a first stage, the GPP time series is derived by computing daily GPP based on Monteith’s radiation use efficiency concept, which accounts for water stress effects to downregulate the maximum light use efficiency (optimal conditions). A suite of MSG products is used, including the daily downwelling shortwave radiation flux (DIDSSF, LSA-203), daily actual evapotranspiration (LSA-351 and LSA-312.3), and reference evapotranspiration (DMETREF, LSA-303). An evaluation of the derived 10-day GPP time series is performed at local scale using ground-based GPP estimates at 8 eddy covariance (EC) towers from the FLUXNET database. The assessment also includes the comparison with other operational EO-based products, such as the 8-day MODIS, 20-day GDMP and daily SMAP at the same EC towers. The results show high correlations (r > 0.70), between the MGPP and EC estimates, which are very similar to those obtained using MODIS, GDMP and SMAP products.

In a second stage, ecosystem monitoring is performed using the multi-resolution analysis (MRA) based on the wavelet transform (WT). MRA-WT provides a temporal decomposition of the original time series, allowing different signal component to be derived by removing the contribution of specific temporal scales. This approach has been extensively used over the past few decades across several applications. The results show a general greening in the central and eastern Sahel region, eastern Africa (Horn of Africa), eastern Spain and Turkey, which is associated with an increase in precipitation along the period. In contrast, localized negative changes are observed in the Senegal region and southern parts of Africa, mainly attributed to precipitation variability during the same period.

How to cite: Martinez, B., Gilabert, M. A., Sánchez-Ruiz, S., Campos-Taberner, M., Jiménez-Guisado, A., and García-Haro, F. J.: GPP from two decades of MSG data for terrestrial ecosystem monitoring over Europe and Africa, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12873, https://doi.org/10.5194/egusphere-egu26-12873, 2026.

EGU26-13139 * | ECS | Orals | GI6.1 | Highlight

A Synergistic Thermal Framework to Classify, Quantify, and Monitor Volcanoes from Space 

Simone Aveni, Marco Laiolo, and Diego Coppola

Volcanic heat flux offers a direct window into subsurface magmatic processes and eruption dynamics, yet its quantification from space remains incomplete. Current satellite-based assessments are largely restricted to high-temperature eruptive activity, resulting in the systematic omission of moderate- and low-temperature sources. We integrate Mid-InfraRed (MIR; 3.5-4.5 μm) and Thermal-InfraRed (TIR; 10-12 μm) satellite observations into a unified analytical framework capable of resolving the full range of volcanic thermal emissions.

We introduce the Total Volcanic Radiative Power (VRPTot), defined as the combined contribution of MIR- and TIR-derived radiative power (VRPMIR + VRPTIR). This approach yields temperature-robust radiative power estimates (within ±20%) over 273-1500 K interval, whereas single-band methods exhibit systematic errors exceeding 90% when applied beyond their operational temperature thresholds. To further characterise thermal behaviour, we define VRPRatio, a dimensionless indicator of volcanic thermal structure that effectively distinguishes hydrothermal, dome-forming, open-vent, and effusive regimes within a common parameter space.

Application of this framework to representative volcanoes demonstrates that inventories relying solely on MIR observations underestimate total thermal output by factors of 2-20 for moderate-temperature systems, indicating that global volcanic heat fluxes may be substantially higher than previously recognised. At Sabancaya volcano, temporal variations in VRPRatio reveal changes in thermal structure several months prior to the November 2016 eruption, signals that are undetectable using single-wavelength approaches.

This transferable methodology enables more accurate assessments of global volcanic heat budgets and enhances the early identification of eruptive transitions, representing a significant advance in satellite-based volcano monitoring. Furthermore, these results resolve long-standing biases in volcanic heat-flux inventories, enhance real-time monitoring capabilities, and have broad implications for volcanology, climatology, and planetary science.

How to cite: Aveni, S., Laiolo, M., and Coppola, D.: A Synergistic Thermal Framework to Classify, Quantify, and Monitor Volcanoes from Space, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13139, https://doi.org/10.5194/egusphere-egu26-13139, 2026.

EGU26-13192 | Orals | GI6.1

Land-Use Classification in a Tropical Wetland: A Comparison of MLC and Machine-Learning Algorithms 

Jacob Nieto, Nelly Lucero Ramírez Serrato, Sergio Armando García Cruzado, Mario Alberto Hernández Hernández, Candelario Peralta Carreta, Graciela Herrera Zamarrón, Selene Olea Olea, Fabiola Doracely Yépez Rincón, Alejandra Cortés, and Guillermo Hernández García

Historical monitoring of land-cover and land-use change provides a means to quantify anthropogenic and atmospheric processes (e.g., floods and droughts) that affect lagoon systems. The Chaschoc-Sejá lagoon system (SLCh-S), located in Tabasco, Mexico, is a natural complex dominated by interconnected lagoons and noted for its high biodiversity, including endemic species. The SLCh-S exhibits strong seasonal dynamics. During the rainy season, it behaves as an interconnected network of water bodies linked by meandering tributaries; extensive flooding occurs, vegetation cover declines, and water bodies display striking color variability. In contrast, during the dry season, interconnections disappear, sediments become exposed, and wet soils and flood-tolerant vegetation emerge along lagoon margins.

 

Although the SLCh-S is undergoing anthropogenic and environmental pressures, the magnitude of these impacts at the regional scale remains poorly understood. Land-use maps derived from remote sensing offer a key first step for large-scale monitoring. However, multiple mapping methods are available, and their performance depends strongly on the characteristics of each study area; therefore, testing is required to identify the most suitable approach.

 

The objective of this study is to evaluate and compare supervised classifiers applied to high-resolution (3 m) satellite imagery to determine which performs best in the region. Two PlanetScope images were analyzed, one from the dry season (March 2024) and one from the rainy season (September 2024). We implemented the traditional Maximum Likelihood Classification (MLC) method and three machine-learning classifiers: Random Forest (RF), Support Vector Machine (SVM), and Random Trees (RT). Classification accuracy was assessed using the Kappa index.

 

Kappa scores were 0.82 for MLC, 0.77 for RF, 0.68 for SVM, and 0.70 for RT. Results indicate that in flat terrain with homogeneous vegetation, agricultural areas, and well-defined water bodies, MLC can effectively classify land use and vegetation, outperforming the tested machine-learning algorithms. Nevertheless, all methods showed limitations in discriminating vegetation with high intra-class spectral variability. The moderate accuracies also highlight the need for post-classification refinement to improve final maps, a step that can be labor-intensive in high temporal-resolution monitoring. Integrating derived variables (e.g., NDVI/NDWI, texture) and complementing accuracy assessment with per-class ROC/AUC metrics (one-vs-rest) is recommended to better characterize class separability.

 

Overall, the study clarifies the strengths and limitations of common classifiers for high-resolution monitoring of tropical wetlands.

How to cite: Nieto, J., Ramírez Serrato, N. L., García Cruzado, S. A., Hernández Hernández, M. A., Peralta Carreta, C., Herrera Zamarrón, G., Olea Olea, S., Yépez Rincón, F. D., Cortés, A., and Hernández García, G.: Land-Use Classification in a Tropical Wetland: A Comparison of MLC and Machine-Learning Algorithms, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13192, https://doi.org/10.5194/egusphere-egu26-13192, 2026.

EGU26-14628 | Posters on site | GI6.1

Current Development Status of Satellite-borne Scanning Array for Hyper-multispectral Radiowave Imaging (SAMRAI) 

Takashi Maeda, Yuta Kobayashi, Nguyen Tat Trung, Yoh Takei, Tsutomu Yano, and Naoya Tomii

Scanning Array for hyper-Multispectral RAdiowave Imaging (SAMRAI) is a passive interferometric radiometer. It realizes ultra-wideband (1-41 GHz) and high-frequency-resolution (27 MHz) microwave spectrum measurement. We believe that SAMRAI is the world's first microwave hyperspectral radiometer.

JAXA has been operating the AMSR series of satellite-borne microwave radiometers for over 30 years, including AMSR3, which was launched in 2025.
However, because the design has remained largely unchanged over this time, various issues have become apparent. In particular, the radio frequency interference (RFI) contaminating the natural-origin signals is a serious problem, and we believe that microwave hyperspectral measurement is essential for identifying and isolating RFI signals. This was a big motivation for developing SAMRAI. In addition, microwave hyperspectral measurement must have new possibilities, such as making it possible to measure the frequency characteristics of the emissivity of the Earth surface.

Development of the satellite-borne SAMRAI is progressing toward launch by 2028. SAMRAI is required to receive natural-origin weak microwave power with high sensitivity over an ultra-wideband range, with an upper frequency limit more than 40 times the lower frequency limit. Furthermore, the microwave power amplified during the reception process must be precisely calibrated to the brightness temperature at the input to the antenna. Developing a new receiver that satisfies all of these requirements posed various challenges, but we have overcome them through design improvements.

Here we present the main design changes made to the SAMRAI ultra-wideband receiver since the start of development in 2021, and the performance improvements achieved through these design changes.

How to cite: Maeda, T., Kobayashi, Y., Trung, N. T., Takei, Y., Yano, T., and Tomii, N.: Current Development Status of Satellite-borne Scanning Array for Hyper-multispectral Radiowave Imaging (SAMRAI), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14628, https://doi.org/10.5194/egusphere-egu26-14628, 2026.

EGU26-15320 | ECS | Orals | GI6.1

Comparison Assessment of Satellite-derived Shorelines using Coastsat Environment and Remote Sensing Technique 

Cherie Pribadi, Riccardo Briganti, and Panagiotis Psimoulis

The coastal zone is one of the most dynamic and high energy systems on Earth, where wind, waves and tides cause geophysical processes such as erosion, deposition and flooding to occur. Monitoring shoreline position is crucial to manage and protect coastal region to safeguard economic and social interest as many people rely on coastal areas for tourism and their livelihoods. Satellite-derived shorelines change rate carried out the significant erosion and accretion along the beaches for assessing the long-term sustainability of coastal development and effective spatial planning. Earth observation (EO) utilisation has been provided moderate spatial resolution (10-30 m) for investigating shoreline movement at regional to global scales. In this study, we delineate the shorelines over three years period of 2022 to 2024 using two distinctive methods – coastsat environment and remote sensing techniques by applying Normalised Difference Water Index (NDWI) algorithm with Sentinel-2 satellite imagery data. Then, we assess the change rates of coastal erosion and accretion using Digital Shoreline Analysis System (DSAS) tool. The significance of shoreline extractions using coastsat environment represent the accretion patterns along the beaches with the average of change rates accounted for 2.54 m/year and 2.65 m/year for Linear Regression Rate (LRR) and End Point Rate (EPR) method, respectively. Meanwhile, the extracted shorelines using NDWI algorithm show the shoreline change rates of -0.87 m/year (LRR) and -0.46 m/year (EPR), which these rates are categorised as a coastal erosion. Moreover, the shoreline distance change rates are also different with the value of 5.27 m (coastsat) and -1.11 m (remote sensing technique), those values were calculated using Net Shoreline Movement (NSM) statistic method. This difference results in shoreline change position might be caused by different process, whereas extracting the shoreline using coastsat that implement the tidal correction and NDWI was applied without tide correction. The other limitation of optical-satellite imagery is the cloud cover can affect the shoreline results followed by its change rates.

How to cite: Pribadi, C., Briganti, R., and Psimoulis, P.: Comparison Assessment of Satellite-derived Shorelines using Coastsat Environment and Remote Sensing Technique, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15320, https://doi.org/10.5194/egusphere-egu26-15320, 2026.

EGU26-17478 | ECS | Posters on site | GI6.1

Comparing Waterline and Water occurrence approaches for satellite‑derived intertidal topography  

Nina Furcic, Simon Déchamps, Edward Salameh, Erwin Bergsma, Frédéric Frappart, and Benoit Laignel
Intertidal zones are situated at the boundary between land and sea and are one of the most important natural buffer zones for the protection of coastal regions, characterized as highly dynamic areas under constant redistribution of sediment. Despite their importance, monitoring the morpho-sedimentary dynamics of intertidal zones is still a challenge. However, satellite measurements enable efficient ways to monitor intertidal areas, providing wide coverage and frequent observation. This study focuses on assessing the performance of two space-based methods in mapping intertidal topography using MultiSpectral (MS) and Synthetic Aperture Radar (SAR) imagery: (i) the waterline method, which uses elevation from waterlines extracted at different tidal stages, with (ii) the water occurrence method, which estimates elevation based on the frequency of inundation of each pixel. To compare the results of these methods, three locations were selected: Bay of Veys, Utah beach and Seine estuary. These sites, located in Normandy region in France, represent different intertidal environments, ranging from a shallow estuarine system to an open beach and an anthropogenically modified intertidal area. DEMs are generated utilizing Sentinel-2 (MS) and Sentinel-1 (SAR) satellites with water level information obtained from two model outputs: the HYbrid Coordinate Ocean Model (HYCOM) and the Finite Element Solution ocean tide model (FES2022). To evaluate the performance of these methods, DEMs were generated using Sentinel-2 data with two different indices (Normalized Difference Water Index - NDWI and Optimized Water Index for Coastal Zones - SCOWI), each of them combined with both water level models. A combination of Sentinel-2 and Sentinel-1 was also tested. All these data combinations were applied to both waterline and water occurrence methods. Compared with LiDAR derived DEMs, preliminary results across all sites show that the waterline method generally achieves Mean Absolute Error (MAE) values in the 0.23 - 0.35 m range, while the water occurrence MAE ranges from 0.33 to 0.57 m. Different intertidal environments and validation data show that both methods have solid performance in different intertidal environments, with opportunities for further improvement. Unlike the waterline method, the water occurrence method can be fully automated, which makes it a promising option for large scale applications.

How to cite: Furcic, N., Déchamps, S., Salameh, E., Bergsma, E., Frappart, F., and Laignel, B.: Comparing Waterline and Water occurrence approaches for satellite‑derived intertidal topography , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17478, https://doi.org/10.5194/egusphere-egu26-17478, 2026.

EGU26-17640 | ECS | Orals | GI6.1

Harmonic decomposition of vegetation indices time series for assessing mining impacts 

Vincent Nwazelibe, Moritz Kirsch, Samuel Thiele, Farid Djeddaoui, Weikang Yu, Richard Gloaguen, and Raimon Tolosana-Delgado

Remotely sensed time-series data provide a powerful tool for environmental monitoring, particularly for assessing heterogeneous spatio-temporal vegetation dynamics in mining environments. Here, we present a new approach, SHABA (Seasonal Harmonic Anomaly Break Analysis), for remotely monitoring the effects of mines on vegetation. SHABA combines Seasonal and Trend decomposition (LOESS), Fast Fourier Transform-based seasonality (e.g., HANTS) and heuristic-based breakpoint detection to identify rapid and long-term vegetation changes. This allows us to quantify browning and greening intensity as deviations from local year-specific periodic and trend behaviour, and identify abrupt but potentially subtle changes (breakpoints). We apply this approach to MODIS EVI data from six mining sites (Aitik, Roșia Poieni, Trident, Lumwana, Carajás, and Vametco). Our results show spatially explicit, significant negative change magnitudes within primary mine footprints, reflecting vegetation loss driven by distinct phases of clearing for infrastructure expansion. Beyond operational boundaries (secondary footprints), change magnitudes are more subtle and exhibit heterogeneous greening–browning patterns, arising from either or a combination of direct mining effects and indirect land-use pressures associated with mine site establishment. SHABA workflow is transferable and can be applied globally to different mines to detect vegetation changes and, when interpreted, supports environmental reporting, impact assessment, and post-mining remediation.

How to cite: Nwazelibe, V., Kirsch, M., Thiele, S., Djeddaoui, F., Yu, W., Gloaguen, R., and Tolosana-Delgado, R.: Harmonic decomposition of vegetation indices time series for assessing mining impacts, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17640, https://doi.org/10.5194/egusphere-egu26-17640, 2026.

EGU26-17996 | Posters on site | GI6.1

From Hyperspectral Unmixing to EUDR Compliance: Scalable Cocoa Traceability in West African Agroforestry Systems 

Gijs Van den Dool, Sacha Malka, and Ellie Jones

Monitoring cocoa farming within complex tropical agroforestry systems remains a significant challenge for Earth Observation, particularly given the EU Deforestation Regulation's requirement for supply chain verification of deforestation-free status at the farm level. In West Africa, distinguishing cocoa trees from forest shade canopies with standard multispectral satellite data is difficult because their spectral signatures are similar.

This study introduces a scalable approach that uses high-resolution hyperspectral imagery from the Wyvern Dragonette satellite constellation to identify cocoa within mixed agroforestry landscapes. The methodology uses Google Earth Engine as the cloud platform and integrates available hyperspectral images, which are limited by frequent cloud cover, with ground-truth data from Abeya’s smallholder supply chain network.

The proposed methodology uses unique spectral 'forest fingerprints' from adjacent native forests to characterise the background canopy. Pixels within farm boundaries that deviate from these forest signatures but correspond to the spectral patterns of known cocoa plantations are identified. These cocoa-specific signatures are subsequently associated with multispectral Sentinel-2 data and pre-trained geospatial foundation models, facilitating cocoa tracking in regions lacking hyperspectral imagery.

This is achieved by utilising the high spectral dimensionality of the Wyvern Dragonette constellation, which captures 31 bands, to resolve sub-pixel mixing between cocoa and forest shade trees that multispectral sensors typically cannot disentangle. These high-fidelity insights are subsequently used to fine-tune pre-trained geospatial foundation models, effectively transferring hyperspectral intelligence to the broader spatial and temporal coverage of the Sentinel-2 archive. This approach demonstrates the potential for emerging satellite constellations to transition from experimental platforms to operational, interdisciplinary monitoring tools that support environmental policy and sustainable supply chain decision-making.

To support validation in data-sparse, smallholder contexts, the framework incorporates participatory field observations when available. Planned farmer questionnaires, aimed at estimating cocoa tree counts and farm-level planting characteristics, will be explored as a complementary source of reference information. These self-reported inputs are intended to provide an independent check on spatial cocoa predictions and help contextualise spectral patterns observed from space. While the availability and completeness of such data may vary, this approach highlights the potential of farmer-generated information to strengthen EO-based monitoring of agroforestry systems.

By focusing on operationally effective modelling choices rather than theoretical optimality, this work outlines a practical pathway for integrating emerging hyperspectral satellite constellations into scalable geospatial workflows. The proposed framework aims to support future assessments of cocoa traceability, EUDR compliance, and sustainable land-use monitoring in tropical agroforestry systems.

How to cite: Van den Dool, G., Malka, S., and Jones, E.: From Hyperspectral Unmixing to EUDR Compliance: Scalable Cocoa Traceability in West African Agroforestry Systems, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17996, https://doi.org/10.5194/egusphere-egu26-17996, 2026.

EGU26-18871 | Posters on site | GI6.1

Spectral properties catalogue of Earth-Venus analogues: Etna example 

Veronika Kopackova-Strnadova and Petra Sedláčková

Volcanic regions provide natural laboratories for studying interactions between surface materials, atmospheric aerosols, and radiative processes on Earth and other planetary bodies. This study combines ground-based gas monitoring, spaceborne hyperspectral imaging, and unsupervised machine learning to characterize the eruptive activity and plume properties of Mount Etna (Italy) and to develop analogs for volcanic processes in the atmosphere of Venus. Etna, Europe’s most active volcano, exhibited persistent activity from 2023 to 2025, dominated by Strombolian explosions, lava fountains, ash plumes, and small lava flows centered on the Southeast Crater Complex.

Key volcanic gas parameters are compiled from Istituto Nazionale di Geofisica e Vulcanologia (INGV) reports into a harmonized, machine-readable dataset. The time series include daily sulfur dioxide flux (SO₂), carbon dioxide flux (CO₂), mean partial pressure of CO₂ (pCO₂), and helium isotope development (He), all of which are fundamental indicators of the state of the magmatic system.

Concurrently, all available Earth Surface Mineral Dust Source Investigation (EMIT) hyperspectral images (350–2500 nm) acquired from the International Space Station over Etna during periods of unrest and eruption are used to characterize the detailed spectral behavior of volcanic surface materials. Radiance and reflectance data cubes are converted to spectral absorption wavelength images to isolate diagnostic absorption features directly related to specific minerals or material types. These products emphasize Fe-bearing silicates, oxides, alteration phases, and other mineral constituents of fresh/weathered lava flows, pyroclastic deposits and volcanic plumes. Unsupervised machine learning classification is then applied to the processed hyperspectral data to derive material and mineral maps without prior training data. For each class, representative spectra (average, minimum, maximum) are computed over the full spectral range to capture characteristic signatures and internal variability, allowing comparison with available spectral libraries (in-house, USGS, ECOSTRESS).

To derive land surface temperature concurrent ECOSTRESS data are selected and analyzed. The ECOSTRESS instrument is a multispectral thermal imaging radiometer that provides high-resolution measurements of surface thermal emission.

The integration of hyperspectral, gas, and thermal datasets provides a promising framework for characterizing volcanic plumes and lava flows. EMIT-based spectral information is combined with concurrent ECOSTRESS thermal observations to derive plume temperatures and discriminate plume types based spectral–compositional signatures. Unsupervised techniques successfully distinguish plumes from the background and identify different plume regimes. Preliminary results indicate that mineral particulates within plumes, including ferric iron (Fe³⁺) phases, can be detected, implying that both gaseous and mineralogical components of volcanic plumes are resolvable in space and time. This is particularly relevant for comparative planetology. The inferred mineralogical composition of terrestrial volcanic plumes may constrain plausible mineral particulates and aerosol types on Venus, yielding testable predictions for the composition and spectral behavior of Venusian volcanic aerosols and mineral dust.

Acknowledgement: The manufacturing of the VenSpec electronics and the preparation of spectral libraries for the EnVision mission in the Czech Republic are funded by ESA PRODEX under contract PEA4000147310.

 

How to cite: Kopackova-Strnadova, V. and Sedláčková, P.: Spectral properties catalogue of Earth-Venus analogues: Etna example, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-18871, https://doi.org/10.5194/egusphere-egu26-18871, 2026.

EGU26-19648 | ECS | Posters on site | GI6.1

Analysing Changes in NDVI: A Long-Term Remote Sensing Approach to Monitor Trends in Plant Phenology of Urban Green Infrastructure 

Franziska Sarah Kudaya, Albert König, and Daniela Fuchs-Hanusch

Climate adaptation strategies for many cities include urban green infrastructure as nature-based solutions due to their potential to mitigate urban heat island effects and reduce surface runoff. However, rising temperatures, drought events and altered precipitation patterns are expected to impact plant phenology by shortening dormancy, resulting in earlier flowering and extended growing seasons. These changes can increase irrigation demand and susceptibility to damage, posing a risk to urban green infrastructure and its ecosystem functions.

In this study, we investigated changes in the growing cycles of urban green infrastructure in four European cities (Birmingham, Paris, Graz, Barcelona) from 1984 to 2024.

The approach is based on monitoring the Normalized Difference Vegetation Index (NDVI) from satellite images to assess long-term trends and analyze the potential effects of climate change on plant phenology in an urban environment. Although analyzing NDVI in urban environments is still relatively new, it is becoming more feasible due to the increased availability of long-term, high-resolution satellite images.

Monthly NDVI values were derived from pre-processed Landsat satellite images to analyze changes in urban green infrastructure and plant phenology. Raster-based pixel counts with an NDVI value above 0.3 were normalized to highlight intra-annual vegetation peaks and seasonal shifts. Temporal trends in vegetation activity were assessed using the non-parametric Mann-Kendall trend test to identify upward or downward trends in the time series. The Theil-Sen Slope Estimator was subsequently applied to determine the magnitude and direction of the detected trends.

The results showed that all four cities expanded their urban green spaces over the past 40 years, with Barcelona exhibiting a particularly substantial increase. Normalized NDVI values revealed an earlier occurrence of peak NDVI and decreases during summer months in certain years, indicating a possible link to drought events. Statistically significant increases in NDVI were observed in March, April, October, and November, indicating both an earlier onset and later offset of the growing season.

Overall the study shows the current changes in plant phenology and developments of urban green infrastructure under climate change. Integrating remote sensing of vegetation with urban water management can support more efficient and adaptive management strategies for irrigating urban green spaces.

How to cite: Kudaya, F. S., König, A., and Fuchs-Hanusch, D.: Analysing Changes in NDVI: A Long-Term Remote Sensing Approach to Monitor Trends in Plant Phenology of Urban Green Infrastructure, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19648, https://doi.org/10.5194/egusphere-egu26-19648, 2026.

EGU26-20279 | Posters on site | GI6.1

MAPEOS: a mobile application for accessing and disseminating space-based remote sensing products for environmental monitoring 

Marco Spina, Carlo Marcocci, Emanuele Pica, Massimo Viola, and Roberto Guardo

The increasing availability of multispectral, thermal and Synthetic Aperture Radar (SAR) observations from satellite and ground-based platforms has significantly enhanced the capability to monitor environmental processes and natural hazards. However, the effective exploitation of Earth Observation products strongly depends on their accessibility, usability and dissemination beyond specialized research environments. In this context, the MAPEOS project aims to develop a mobile application designed to facilitate access to and dissemination of remote sensing products for environmental monitoring, bridging the gap between advanced Earth Observation infrastructures and end users.

MAPEOS is conceived as a cross-platform mobile application that disseminates scientific data and value-added products generated by the Platform for Earth Observation from Space (PEOS), a national e-infrastructure developed within the Italian “Monitoring Earth’s Evolution and Tectonics” (MEET) project, funded by the National Recovery and Resilience Plan (PNRR – Next Generation EU). PEOS is coordinated within the activities of the INGV Center for Space Observations of Earth (COS) and contributes to the European Plate Observing System (EPOS) research infrastructure. While PEOS provides the processing, integration and management of heterogeneous remote sensing datasets, MAPEOS focuses on user-oriented delivery of selected products, emphasizing intuitive visualization, rapid access and effective communication of environmental information.

The mobile application supports the visualization of key Earth Observation products relevant to environmental monitoring and natural hazard assessment. These include ground deformation derived from SAR interferometry, surface temperature and environmental parameters from multispectral and thermal imagery, volcanic cloud properties and SO₂ and ash emissions, as well as a range of space weather products derived from satellite observations and ground-based measurements. In particular, MAPEOS aims to disseminate information related to geomagnetic activity, ionospheric disturbances and space weather conditions that can affect technological systems and the near-Earth environment, providing an integrated view of solid Earth, atmospheric and space-related processes.

A central aspect of MAPEOS is its ability to exploit harmonized and fused products generated within PEOS, integrating spectral, spatial and temporal information from multiple sensors and platforms. The application accesses data through standardized application programming interfaces (APIs) compliant with OGC standards, OpenAPI specifications and the EPOS-DCAT-AP profile, ensuring interoperability, scalability and alignment with FAIR principles. This architecture allows the mobile application to remain lightweight while providing near–real-time access to updated remote sensing and space weather products.

MAPEOS is designed for a broad range of users, including researchers, students, civil protection operators and the general public. By lowering technical barriers and enabling mobile access to Earth Observation and space weather information, the application supports knowledge transfer, outreach activities and increased awareness of environmental processes and natural hazards.

This contribution presents the design concept and current development status of the MAPEOS mobile application, highlighting the role of mobile technologies in enhancing the accessibility and societal impact of space-based remote sensing products for environmental monitoring and decision-support applications within national and European frameworks.

How to cite: Spina, M., Marcocci, C., Pica, E., Viola, M., and Guardo, R.: MAPEOS: a mobile application for accessing and disseminating space-based remote sensing products for environmental monitoring, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20279, https://doi.org/10.5194/egusphere-egu26-20279, 2026.

EGU26-20448 | Posters on site | GI6.1

A Lightweight UAV-based Spectroscopic System for Water Quality Monitoring in Mining-Impacted Environments: Setup, Data Processing, and Validation 

Martin Kýhos, Jan Jelének, Barbora Kořínková, Giannis Zabokas, Martín López del Río, Sergio Tenorio Matanzo, and Veronika Kopačková-Strnadová

Monitoring water quality in areas affected by mining activities requires high-spatial and temporal resolution data, which remains a challenge for traditional satellite and ground-based methods. We present a novel, cost-effective instrumental setup for water surface reflectance measurements using a miniature light-weight Ocean Optics STS-VIS microspectrometer (40 x 42 x 24 mm; 337–823 nm; 1.2 nm spectral resolution; 1024 bands). The sensor was mounted on the DJI Phantom 3 Advanced UAV using a custom-developed, 3D-printed holder to ensure stability and precise nadir orientation. With a field of view (FOV) of 25° and an operational flight altitude of 3 m, the system achieved a spatial resolution (ground footprint) of 1.2 m per measurement point, allowing for precise targeting of narrow water bodies. The system was used across three diverse mining regions: the Chalkidiki Peninsula and Kirki (Greece), and Andalusia (Spain).

To derive accurate reflectance from raw intensity data, a standardized calibration protocol was established, involving dark spectrum subtraction and reference measurements using a Spectralon panel (Spectral Evolution; 100% reflectance). Flights were conducted manually to minimize propeller propeller-induced surface turbulence, following standardized patterns (longitudinal and diagonal for streams; sun-relative for water bodies).

The processing workflow addresses the high volume of raw data (up to 400 spectra per site). We implemented a smoothing pipeline and filtration:

(1) application of Savitzky-Golay filters (SGF) with a 2nd-degree polynomial and varying window sizes (66, 99, 132),

(2) statistical outlier removal based on +/-1.5 standard deviations,

(3) visual inspection eliminating interference from bank vegetation or rocks above the water.

Based on our analysis, the SGF window size of 99 was selected as optimal. While the window size 66 left significant residual noise and the window size of 132 caused the loss of critical spectral absorption features, the window size of 99 provided sufficient noise reduction while preserving the integrity of the spectral signal.

The final averaged spectra were correlated with water sample laboratory analyses using Partial Least Squares Regression (PLSR). Our results identified key wavelengths sensitive to specific mining-related water quality parameters. This study demonstrates that the proposed UAV-spectrometer integration provides a robust, flexible, and high-precision alternative for monitoring contaminated aquatic systems in logistically challenging environments.

The presented analysis was conducted under the support of the EC through the MultiMiner project, funded under the European Union’s Horizon Europe research and innovation programme (Grant Agreement No. 10109137474), and under the support of the MINEYE project, funded under the European Union’s Horizon Europe research and innovation programme (Grant Agreement No. 101138456).

How to cite: Kýhos, M., Jelének, J., Kořínková, B., Zabokas, G., López del Río, M., Tenorio Matanzo, S., and Kopačková-Strnadová, V.: A Lightweight UAV-based Spectroscopic System for Water Quality Monitoring in Mining-Impacted Environments: Setup, Data Processing, and Validation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20448, https://doi.org/10.5194/egusphere-egu26-20448, 2026.

EGU26-21444 | ECS | Posters on site | GI6.1

National Scale Estimation of Methane Emissions from Rice Paddies in South Korea Using UAV and Sentinel-2 Time Series Data 

Yongho Song, Cholho Song, Sol-E Choi, and Woo-kyun Lee

Methane (CH₄) has a global warming potential approximately 20 times greater than that of carbon dioxide and is a major greenhouse gas emitted from rice paddies, making systematic emission management essential for achieving carbon neutrality. In South Korea, national greenhouse gas statistics are currently derived using IPCC Tier 1 and Tier 2 emission factor–based approaches, which have limitations in accounting for region-specific rice cultivation environments and management practices. Therefore, spatially detailed estimation of methane emissions is required. To address this need, this study first estimated methane emissions using time series unmanned aerial vehicle (UAV) observations and subsequently scaled up the approach using Sentinel-2 satellite time-series imagery to quantify methane emissions from rice paddies across South Korea.

Rice paddies were identified nationwide using a phenology-based classification approach derived from Enhanced Vegetation Index 2 (EVI2) time-series composites. Sentinel-2 data were processed on the Google Earth Engine platform as five-year averaged datasets from 2020 to 2024, with 15-20 day intervals during the rice growing season, considering cloud conditions to ensure image quality. Spatial and temporal consistency was achieved through cloud masking and median compositing. To reflect regional heterogeneity in rice growth processes, region-specific rice cultivar information and growth-stage timing at the municipal level were incorporated into the analysis.

For national-scale methane estimation, the temporal behavior of Sentinel-2 derived EVI2 was evaluated through comparison with UAV-derived EVI2 observations acquired at key rice growth stages. Quantitative agreement between satellite- and UAV-based EVI2 values was limited during the early growth stages, whereas consistent temporal trends were observed after the heading stage. Based on these findings, Sentinel-2 EVI2 variables observed after the heading stage were selected as explanatory variables for the methane emission model, and UAV-based methane flux estimates were used as reference data.

The resulting empirical regression model was applied to all identified rice paddies nationwide to estimate methane emissions at both the parcel and administrative unit scales. The spatial distribution of estimated emissions exhibited pronounced regional variability, reflecting differences in rice cultivation area and growth conditions. Absolute emission estimates were slightly lower than those reported in some previous studies, a result attributed to mixed-pixel effects inherent in moderate-resolution satellite imagery. Despite this difference, the spatial patterns of methane emissions and the relative ranking among regions were generally consistent with results from comparable rice methane studies and national statistics.

This study demonstrates the applicability of a Tier 2.5 level methane emission estimation approach that integrates rice growth information derived from satellite time-series data. The proposed framework provides a scalable and cost-effective pathway for improving national greenhouse gas inventories and supporting the development of region-specific mitigation strategies for methane emissions from rice cultivation.

Acknowledgement:
This work was supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF), funded by the Ministry of Education (RS-2021-NR060142), and by the BK21 FOUR program (Grant No. 4120200313708), funded by the National Research Foundation of Korea (NRF).

How to cite: Song, Y., Song, C., Choi, S.-E., and Lee, W.: National Scale Estimation of Methane Emissions from Rice Paddies in South Korea Using UAV and Sentinel-2 Time Series Data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21444, https://doi.org/10.5194/egusphere-egu26-21444, 2026.

Urban heat risk assessments increasingly require land surface temperature (LST) and near-surface air temperature at spatial scales that resolve microclimatic drivers such as material heterogeneity, shading, and complex terrain. While satellite thermal products and stationary air temperature observations provide essential regional and temporal context, their spatial resolution and coverage, as well as satellite revisit frequency, limit the quantification of surface thermal variability within urban blocks and campus-scale environments. Unmanned aerial vehicle (UAV) thermal imagery can bridge this scale gap, but quantitative LST retrieval remains sensitive to radiometric calibration, emissivity assumptions, local viewing geometry, geolocation accuracy, and acquisition-time atmospheric conditions.

This contribution develops and demonstrates a reproducible UAV thermal remote sensing workflow that converts raw thermal imagery into georeferenced LST mosaics over complex urban surfaces. Using a DJI Matrice 4T thermal sensor over a university campus in Sheffield, UK, thermal data were collected through multiple field surveys combining UAV flights with ground measurements collected alongside the flights. UAV flights were conducted in late June 2025, with flight planning targeting approximately 80% forward and side overlap. Raw thermal imagery derived from UAV was batch-converted using documented acquisition parameters informed by on-site conditions. Key factors include target distance, relative humidity, emissivity, and reflected apparent temperature,  applied consistently within each survey to support cross-frame comparability.  This research: (1) converts raw thermal imagery to georeferenced thermal outputs using ground-informed acquisition parameters (i.e. distance, humidity, emissivity, and reflected apparent temperature) to stabilise cross-frame temperature consistency; (2) reduces spatial distortions through co-registration with high-resolution basemaps, with a digital terrain model (DTM) used as an additional terrain reference; (3) accounts for surface emissivity variability by integrating land use/land cover and material proxies derived from complementary geospatial datasets, with high-resolution RGB orthomosaics used to derive land cover or material proxies (e.g., vegetation and pavements) that inform thermal processing parameters and support consistent interpretation of microscale thermal patterns.

The workflow delivers thermal remote sensing products at centimetre-level ground sampling distances and is designed to be transferable to other urban sites using standard UAV surveys and widely available geospatial datasets. By foregrounding calibration, emissivity handling, and quality control, this study strengthens the methodological basis for integrating UAV thermal observations into environmental remote sensing in urban settings, enabling more robust cross-scale interpretation of urban thermal patterns and supporting evidence-based decision making.

How to cite: Wang, J.: UAV thermal remote sensing for land surface temperature mapping in complex urban environments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21586, https://doi.org/10.5194/egusphere-egu26-21586, 2026.

EGU26-22137 | Orals | GI6.1

Multi-Branch Convolutional Neural Networks for Volcanic Activity Classification Using Thermal Imagery (Cotopaxi and El Reventador volcanoes) 

Silvia Vallejo, Diana Mosquera, Francisco Gallegos, Pedro Merino, Fernanda Naranjo, and Gerardo Pino

Over the last 25 years, five volcanoes have erupted on mainland Ecuador, generating eruptive columns, pyroclastic density currents, lava flows, etc. Currently, El Reventador and Sangay are erupting and are being monitored by the Instituto Geofísico of the Escuela Politécnica Nacional (IGEPN) using different techniques, including thermal surveillance. The volcanic products emitted by these volcanoes are identified through thermal and visual image analysis. The timely identification of these products can greatly influence decision-making by authorities and the response of vulnerable populations.

This study presents a novel approach to the automated classification of volcanic states using thermal imagery from multiple Ecuadorian volcanoes, acquired by the IGEPN. We developed a Multi-Branch Convolutional Neural Network architecture that processes three-dimensional tensor representations of thermal data to distinguish between clear conditions, cloudy conditions, emission events, and lava flow events. The system processes raw FLIR camera images (.fff format) through a pipeline that includes metadata extraction, thermal analysis, and classification. Our architecture utilizes three parallel branches processing base thermal information, edge detection features, and volcano-specific thermal thresholds simultaneously.

The model was trained and validated on a dataset of more than 10,000 thermal images from two active Ecuadorian volcanoes: Cotopaxi (7,024 images) and Reventador (3,536 images). The dataset encompasses four volcanic states: cloudy conditions, emission events, clear conditions, and lava flow events. Our multi-volcano approach incorporates volcano-specific thermal threshold parameters, recognizing the distinct thermal characteristics of different volcanic systems. The model achieved robust performance with 94.74% validation accuracy and 94.58% training accuracy across all volcanic states and locations. Per-class validation performance demonstrates excellent discrimination capability: <95% for clear conditions, <96% for cloudy conditions, <94% for emission events, and <90% for lava flow events. The confusion matrix reveals minimal inter-class confusion, indicating the model's ability to distinguish between complex volcanic phenomena. This approach addresses key challenges in manual analysis of thermal imagery while providing a scalable framework that can be adapted to different volcanic systems and integrated into existing monitoring networks.

How to cite: Vallejo, S., Mosquera, D., Gallegos, F., Merino, P., Naranjo, F., and Pino, G.: Multi-Branch Convolutional Neural Networks for Volcanic Activity Classification Using Thermal Imagery (Cotopaxi and El Reventador volcanoes), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22137, https://doi.org/10.5194/egusphere-egu26-22137, 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.

EGU26-671 | ECS | Orals | AS3.38

High-resolution measurement-based methane quantification from beef cattle feedlots to improve agricultural GHG inventories 

Sushree Sangita Dash, Trevor W. Coates, and Chandra A. Madramootoo

Methane (CH4) emissions from livestock production remain one of the largest and most uncertain components of national greenhouse gas inventories, largely because direct measurements at operational facilities are limited. This measurement gap constrains the accuracy of agricultural CH4 estimates and the development of effective mitigation strategies. Strengthening the empirical basis for these inventories is therefore essential. Emerging close-range tools, such as uncrewed aerial vehicle (UAV) plume-sampling systems, can enhance monitoring, reporting, and verification (MRV) by providing high-resolution, facility-level observations.

To evaluate this approach, this study conducted a five-day field campaign at a commercial cattle feedlot in southern Alberta, Canada, housing approximately 28,000 cattle. UAV plume sampling was deployed alongside continuous CH4 measurements from an open-path laser (OPL) to estimate CH4 emission rate downwind of the facility. For both techniques, emission rates were derived using inverse dispersion modeling, for a direct comparison of performance and assessing the extent to which UAV-based sampling can complement established ground-based flux measurements.

Uncrewed aerial vehicle-derived CH4 emission rates varied from 149 to 392 g head-1 day-1 (mean ± SE: 280 ± 22), in near-perfect agreement with OPL-derived emissions of 152-438 g head-1 day-1 (280 ± 22). Daily mean emissions differed by only 0.08% during overlapping sampling periods, and statistical distributions were highly consistent across methods. Hour-to-hour variability reflected transient atmospheric dynamics and associated changes in plume dispersion, rather than methodological bias. UAV flights also revealed spatial plume gradients not captured by the fixed OPL geometry, and consistent hourly emission estimates were found when UAV flights collected at least four usable plume samples per hour. Performance declined under very low-wind or highly turbulent conditions, clarifying key operational constraints for future deployments.

Overall, these findings demonstrate that UAV-based plume sampling can provide CH4 emission estimates consistent with established ground-based systems, providing a validated pathway for quantifying emissions from commercial feedlots. The approach aligns with the Integrated Global Greenhouse Gas Information System (IG3IS) good-practice principles and provides empirical information that can improve IPCC Tier 2 emission factors for open-lot beef operations.

How to cite: Dash, S. S., Coates, T. W., and Madramootoo, C. A.: High-resolution measurement-based methane quantification from beef cattle feedlots to improve agricultural GHG inventories, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-671, https://doi.org/10.5194/egusphere-egu26-671, 2026.

EGU26-2527 | ECS | Orals | AS3.38

Investigating Regional Halocarbon Emissions: The Seoul Tracer Release Experiment 

Michelle Jessy Müller, Martin K. Vollmer, Stephan Henne, Jaegeun Yun, Haklim Choi, Sunyoung Park, Lukas Emmenegger, and Stefan Reimann

Hydrofluorocarbons (HFCs) are used as refrigerants, propellants or insulating foams. They don’t deplete the ozone layer like their predecessors, (hydro)chlorofluorocarbons ((H)CFCs). However, HFCs are still potent greenhouse gases and are regulated under the Kyoto Protocol (1997) and, more recently, the Kigali Amendment to the Montreal Protocol. The Kigali amendment targets reductions in HFC production and consumption over the coming decades.1, 2 Observing halogenated substances in the atmosphere provides an independent means to verify compliance with these international treaties. From these observations, regional and global emission estimates can be obtained by combining them with atmospheric modelling or using a reference tracer with known emissions.3, 4 Due to rapid industrialization and high demand for refrigeration and air conditioning, the eastern Asian region contributes significantly to global HFC emissions. Therefore, it is crucial to understand the emission patterns in this region to assess global compliance.

We have conducted a large-scale controlled-release tracer experiment to estimate regional halocarbon emissions of the greater Seoul metropolitan area (South Korea). Ethyl fluoride (HFC-161)5 and hexafluorobutane (HFO-1336mzzE), which are virtually absent in the background atmosphere, were released at one location in the City of Seoul. Release times were selected to align with favorable meteorological conditions that allowed air masses to reach the AGAGE station Gosan (Jeju Island, 490 km south of Seoul). The site is equipped with an instrument for in-situ halocarbon measurements. Intermediately located along the path of air mass transport, sites at the Global Atmosphere Watch (GAW) Observatory Anmyeondo and Mokpo National University (138 km and 320 km from Seoul, respectively) were used for additional flask sampling. The atmospheric transport model FLEXPART6 was used to forecast the tracer plume's trajectory and dispersion, and the release and sampling times were adjusted accordingly.

During two releases in November 2024 and April 2025, both tracers were detected at the flask sampling sites Anmyeondo GAW Observatory and Mokpo National University, as well as at Gosan station. The measurements show a strong correlation of our tracer substances with various HFCs. Preliminary emission estimates for the greater Seoul metropolitan area are derived using the tracer ratio method, and its limitations are discussed. Finally, a comparison to a full regional inversion, based on the continuous observations at Gosan, is conducted.

References

[1] Kyoto Protocol to the United Nations Framework Convention on Climate Change. adopted on December 11th, 1997; Kyoto, 1998, 1-22.

[2] Kigali Amendment to the Montreal Protocol on Substances that Deplete the Ozone Layer. adopted on October 15th, 2016; United Nations, Kigali.

[3] Matt Rigby, Sunyoung Park, Takuya Saito, Luke M. Western, Alison L. Redington, et al., Nature, 2019, 569 (7757), 546-550.

[4] Peter G. Simmonds, Matthew Rigby, Alistair J. Manning, Sunyoung Park, Kieran M. Stanley, et al., Atmospheric Chemistry and Physics 2020, 20 (12), 7271-7290.

[5] Dominique Rust, Martin K. Vollmer, Stephan Henne, Arnoud Frumau, Pim van den Bulk, et al., Nature, 2024, 633, 96-100.

[6] Ignacio Pisso, Espen Sollum, Henrik Grythe, Nina I. Kristiansen, Massimo Cassiani, et al., Geoscientific Model Development, 2019, 12 (12), 4955-4997.

How to cite: Müller, M. J., Vollmer, M. K., Henne, S., Yun, J., Choi, H., Park, S., Emmenegger, L., and Reimann, S.: Investigating Regional Halocarbon Emissions: The Seoul Tracer Release Experiment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2527, https://doi.org/10.5194/egusphere-egu26-2527, 2026.

EGU26-2643 | Orals | AS3.38

Unveiling Carbon Sequestration Dynamics in Bamboo Forests, China: An Observation-Based Approach Using Atmospheric Tracers 

Shuangxi Fang, Oksana Tarasova, Yanxia Li, Jocelyn Turnbull, Yi Lin, Gordon Brailsford, and Sara Mikaloff-Fletcher

Bamboo, a perennial grass species, exhibits rapid growth rates surpassing many native trees, offering substantial potential for atmospheric carbon capture and subsequent sequestration into durable products. Despite this promise, the carbon sequestration capacity of bamboo forests and its variability under different land management practices and environmental conditions remain underexplored. This study examines carbon sequestration in a representative bamboo forest in Anji, eastern China, employing a novel observation-based approach utilizing multiple atmospheric tracers (CO₂, CO, and ¹⁴C-CO₂) measurements to attribute fluxes accurately. The study also includes regular biomass inventory to be able to compare CO2 fluxes between two approaches. Departing from conventional inventory-based estimates of carbon emissions and uptakes, observations-based method yields detailed insights into individual carbon-cycle processes within bamboo ecosystems and identifies the most effective tracers for quantifying regional CO₂ fluxes. Leveraging high-resolution atmospheric CO₂ observations, coupled with advanced modeling systems and analytical tools—including machine learning techniques to reconstruct and correct prior Net Ecosystem Exchange (NEE) fluxes for the bamboo forest—we derive carbon fluxes while accounting for variations in management strategies and environmental factors. These findings enhance our understanding of bamboo's role in global carbon mitigation, informing sustainable forestry practices and climate policy. This work highlights the transformative potential of tracer-based methodologies for precise, scalable carbon flux assessments in managed ecosystems.

The study is supported by the Quadrature Climate Foundation (Grant No. 01-21-000133).

How to cite: Fang, S., Tarasova, O., Li, Y., Turnbull, J., Lin, Y., Brailsford, G., and Mikaloff-Fletcher, S.: Unveiling Carbon Sequestration Dynamics in Bamboo Forests, China: An Observation-Based Approach Using Atmospheric Tracers, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2643, https://doi.org/10.5194/egusphere-egu26-2643, 2026.

EGU26-2748 | Orals | AS3.38

Design, operation, and insights from Zurich’s mid- and low-cost ICOS Cities CO2 sensor network 

Lukas Emmenegger, Luce Creman, Andrea Fischer, Stuart K. Grange, Christoph Hüglin, Pascal Rubli, and Dominik Brunner

Zurich aims for net-zero direct greenhouse gas emissions by 2040, a target supported by 75 % of voters. Progress is tracked through a detailed CO2 inventory covering energy, transport, industry, and waste. Under the European ICOS Cities project, a monitoring program was launched using two approaches: (i) a network of mid- and low-cost CO2 sensors combined with atmospheric inverse modeling, and (ii) CO2 flux measurements from an eddy-covariance system on a city-center high-rise building, paired with footprint modeling.

Here, we focus on the mid-cost (ZiCOS-M) and low-cost (ZiCOS-L) NDIR (nondispersive infrared) CO2 networks, which were both operational for at least 3 years since 2022.

ZiCOS-M consists of 26 monitoring sites, 21 in the city and 5 outside the urban area. Daily calibrations using two reference gas cylinders, and corrections of the sensors’ spectroscopic response to water vapour were performed. The hourly mean root mean squared error (RMSE) was 0.98 ppm (0.46 - 1.5 ppm) and the mean bias ranged between 0.72 and 0.66 ppm compared to parallel measurements with a high-precision reference gas analyser for a period of 2 weeks or more. CO2 concentrations in the city were highly variable with site means ranging from 434 to 460 ppm, and Zurich’s mean urban CO2 increment was 15.4 ppm above the regional background.

ZiCOS-L consists of 56 sites with paired sensors. The sensors require in-field training for model calibration before deployment and further post-processing steps to account for drift and outliers. After data processing, the hourly RMSE was 13.6±1.4 ppm, and the mean bias 0.75±1.67 ppm when validated against parallel reference measurements from ZiCOS-M. CO2 concentrations were highly variable with site means in Zurich ranging from 438 to 465 ppm, reflecting mainly the influence of sources in the nearby surroundings. Vegetation (mainly grassland) amplified the morning concentration on average in summer by up to 20 ppm due to ecosystem respiration, while heavy traffic increased the morning rush hour concentration by 15 ppm. Despite its lower measurement accuracy, the ZiCOS-L network enables the study of concentration dynamics at a spatial and temporal scale that is not accessible by any other means.

The ZiCOS-M data was extensively used to derive top-down CO2 emissions. Similar modelling activities are currently ongoing with the ZiCOS-L data, and both are compared to emissions derived from the eddy covariance system and to the city's emission inventory.

 

Grange SK, … Emmenegger L, The ZiCOS-M CO2 sensor network: measurement performance and CO2 variability across Zurich. https://doi.org/10.5194/acp-25-2781-2025.

Creman L, … Bernet L, The Zurich Low-cost CO2 sensor network (ZiCOS-L): data processing, performance assessment and analysis of spatial and temporal CO2 dynamics. https://doi.org/10.5194/egusphere-2025-3425

Brunner D, … Emmenegger L, Building-resolving simulations of anthropogenic and biospheric CO2 in the city of Zurich with GRAMM/GRAL. https://doi.org/10.5194/acp-25-14279-2025.

Hilland R, … Christen A, Sectoral attribution of greenhouse gas and pollutant emissions using multi-species eddy covariance on a tall tower in Zurich, Switzerland. https://doi.org/10.5194/acp-25-14279-2025.

Ponomarev N, … Brunner D, Estimation of CO2 fluxes in the cities of Zurich and Paris using the ICON-ART CTDAS inverse modelling framework. https://doi.org/10.5194/egusphere-2025-3668.

How to cite: Emmenegger, L., Creman, L., Fischer, A., Grange, S. K., Hüglin, C., Rubli, P., and Brunner, D.: Design, operation, and insights from Zurich’s mid- and low-cost ICOS Cities CO2 sensor network, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2748, https://doi.org/10.5194/egusphere-egu26-2748, 2026.

EGU26-2817 | ECS | Orals | AS3.38

Concurrent data assimilation of methane concentrations and fluxes  

Niklas Becker, Niels Heinrich Keil, Valentin Bruch, and Andrea Kaiser-Weiss

We use atmospheric inverse modelling to provide observation-based estimates of methane emissions at the national scale in Europe. We apply the numerical weather prediction model ICON-ART to obtain an ensemble of methane concentrations by varying the meteorology, the lateral boundary conditions and emission fields. By comparing to ground based observations of the ICOS network, we employ a 4D LETKF to assimilate both the concentrations and emissions concurrently. We create an ensemble of emissions in two ways: We can perturb the underlying emission field with a gaussian random field, or we can separate it into regions and economic sectors and scale these. We compare the two approaches and the resulting emission estimates to national greenhouse gas inventories and synthesis inversion results with a focus on Germany. The first results are presented for 2021 and we identify a considerable mismatch with the reported emissions in central Europe.

How to cite: Becker, N., Keil, N. H., Bruch, V., and Kaiser-Weiss, A.: Concurrent data assimilation of methane concentrations and fluxes , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2817, https://doi.org/10.5194/egusphere-egu26-2817, 2026.

EGU26-3366 | Posters on site | AS3.38

Characteristics of CO2 and CH4 from different emission sources using mobile measurements and stable carbon isotope analysis 

Hyeongseok Choi, Jongbyeok Jun, Sunran Lee, Sumin Kim, and Yongjoo Choi

Achieving effective greenhouse gases (GHGs) mitigation policy requires accurate quantification of contribution from each emission source based on in-situ measurements. In this study, we investigated the spatial distribution of CO2 and CH4 emitted from different emission sources by conducting mobile measurements using a GLA331-GGA analyzer (ABB–LGR Inc.) mounted on a vehicle. We conducted seven mobile measurements in spring (N = 3), summer (N = 2), and fall (N = 2) over Seoul Metropolitan Area (SMA) in 2025. By comparing the correlation between two GHGs from various emission sources, we selected representative sites including livestock facilities (cattle and swine barns), industrial complexes, urban, wastewater treatment plants, LNG power plants, rural areas. Background GHGs concentrations were defined as the daily 5th percentile for each measurement day, and correlations between enhancements (ΔCO2 and ΔCH4) were assessed. Along with real time measurements, stable carbon isotopes samplings were also conducted to provide complementary constraints on concentration variability and the contributions of end-member of each emission source. For stable isotope measurements, two ambient air samples were collected per site using canisters (Entech, Simi Valley, CA, USA) and analyzed with Picarro G2131-i for δ13C–CO213C) and Picarro G2132-i for δ13C–CH413CH4). Strong co-variability between the two GHGs was observed at several emission sources and seasons, including springtime cattle barns (R = 0.75), LNG power plants (R = 0.83), industrial complexes (R = 0.74), and swine barns (R = 0.64); summertime cattle barns (R = 0.66) and LNG power plants (R = 0.67); and fall industrial complexes (R = 0.70) and cattle barns (R = 0.97). These correlations suggested that CO2 and CH4 were likely emitted concurrently from shared sources or similar emission activities in SMA region. The observed δ13C values ranged from −8.2‰ to −12.5‰, while δ13CH4 ranged from −47.2‰ to −48.6‰. Seasonal mean δ13C values were −11.2‰ in spring, −9.2‰ in summer, and −10.1‰ in fall, consistent with a summertime influence from enhanced biospheric respiration, with the most depleted values occurring in spring. In contrast, δ13CH4 exhibited relatively small seasonal variability, as indicated by the coefficient of variation (sd/mean; 0.004 in spring, 0.013 in summer, and 0.012 in fall), but still provided useful constraints on source attribution. In addition, a Bayesian isotope mixing model (the ‘simmr’ package in R) was applied to quantify relative source contributions indicating that coal combustion contributed most strongly to δ13C, whereas wastewater treatment and natural gas were the dominant contributors to δ13CH4.

How to cite: Choi, H., Jun, J., Lee, S., Kim, S., and Choi, Y.: Characteristics of CO2 and CH4 from different emission sources using mobile measurements and stable carbon isotope analysis, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3366, https://doi.org/10.5194/egusphere-egu26-3366, 2026.

EGU26-3437 | ECS | Orals | AS3.38

Development of an Ensemble-Based Data-Assimilation System for CO2 Fluxes Using ICON-ART 

Jakob Böttcher, Niklas Becker, Andrea Kaiser-Weiss, and Maya Harms

Observation based quantification of surface CO2 fluxes relies on the consistent integration of atmospheric observations with numerical transport models. We present the development and demonstration of an ensemble-based data assimilation system that couples atmospheric CO2 observations to the ICON-ART modeling framework using a Local Ensemble Transform Kalman Filter (LETKF).

 

Starting with a flux estimate provided by CarbonTracker Europe High-Resolution we start with a dynamic model with hourly resolution with a focus on fluxes in Europe for 2021. We then create an ensemble of perturbed prior fluxes within assumed uncertainties using prescribed spatial and temporal correlation structures. We simulate the transport of these ensemble members in ICON-ART in limited area mode, while varying the meteorological conditions to represent meteorological uncertainties. Subsequently, we use the LETKF to update the state vector of concentrations and CO2 fluxes daily, resulting in an posterior estimate of surface CO2 fluxes over Europe. 

 

This work provides the foundation for an ICON-ART-based CO2 flux assimilation system and establishes a technical basis for future extensions toward longer assimilation periods, refined error modeling, and the assimilation of anthropogenic emission signals.

How to cite: Böttcher, J., Becker, N., Kaiser-Weiss, A., and Harms, M.: Development of an Ensemble-Based Data-Assimilation System for CO2 Fluxes Using ICON-ART, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3437, https://doi.org/10.5194/egusphere-egu26-3437, 2026.

In this research, we propose a simple and effective method for gas analysis of semiconductor and display industries. To achieve this, residual gas analyzer (RGA) was adopted and two high-global warming potential (GWP) gases such as CF4 and NF3 commonly used in industrial application were focused. The experiment was conducted in four key steps: identifying gas species using optical emission spectroscopy (OES), calibrating RGA with a quadrupole mass spectrometer (QMS), constructing a five-point calibration graph to correlate RGA and Fourier-transform infrared spectroscopy (FT-IR) data, and estimating the concentration of unknown samples using the calibration graph. The results under plasma-on conditions demonstrated correlation and accuracy, confirming the reliability of our approach. In other words, the method effectively captured the relationship between RGA intensity and gas concentration, providing valuable insights into concentration trends. Thus, our approach serves as a useful tool for estimating gas concentrations and understanding the correlation between RGA intensity and gas composition.

 

Reference

[1] B. G. Jeong, S. H. Park, D. H. Goh, and B. J. Lee, Metrology 5 (2025) 60

How to cite: Jeong, B. G.: Real-Time Monitoring and Quantification of Fluorinated Greenhouse Gases in Semiconductor/Display Manufacturing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4566, https://doi.org/10.5194/egusphere-egu26-4566, 2026.

The semiconductor and display industries are significant sources of fluorinated greenhouse gas (F-GHG) emissions in the electronics, making accurate emission estimation essential for addressing climate change. The Republic of Korea, a leading country in the semiconductor and display industries, requires precise evaluation of the environmental impact of these industries due to its global competitiveness. Currently, The Republic of Korea relies on default emission factors provided by the 2006 IPCC guidelines for estimating F-GHG emissions. However, this approach does not account for the latest mitigation technologies implemented in Republic of Korea, resulting in a conservative overestimation of actual F-GHG emissions. To address this issue, this study conducted direct measurements of F-GHG emissions from semiconductor manufacturing processes in facilities equipped with advanced mitigation technologies. By employing state-of-the-art measurement methods, the study evaluated the use rate of gas (Ui) and generation rate of by-product gas (Bbyproduct, Bi) and compared the results with the default emission factors provided by IPCC G/L (2006 and 2019). Moreover, based on derived country-specific emission factors (Tier 3b), GHG emissions were estimated and compared with tier-based methodologies using 2006 and 2019 IPCC G/L default factors (Tier 2a, 2b, 2c and 3a). The finding highlights the need for developing country-specific emission factors and contribute to the establishment of precise, data-driven policies for reducing GHG emissions in Republic of Korea’s electronics industry. Furthermore, this research serves as valuable reference for other countries aiming to refine their emission estimates with country-specific data and technological advancements, ultimately contributing to global efforts towards carbon neutrality.

How to cite: Inkwon, J. and Bong-Jae, L.: Comparative Analysis of F-GHGs Emission Estimates between IPCC Default Factors and Measurement-based Korea-specific Emission Factors in Semiconductor Manufacturing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-4570, https://doi.org/10.5194/egusphere-egu26-4570, 2026.

EGU26-5198 | ECS | Orals | AS3.38

Monitoring urban atmospheric CO2 plumes from space: sensitivity to urban physics and scale effects over Paris 

Alohotsy Rafalimanana, Thomas Lauvaux, Charbel Abdallah, Mali Chariot, Michel Ramonet, Josselin Doc, Olivier Laurent, Morgan Lopez, Anja Raznjevic, Maarten Krol, Leena Järvi, Leslie David, Olivier Sanchez, Andreas Christen, Dana Looschelders, Laura Bignotti, Benjamin Loubet, Sue Grimmond, and William Morrison

Quantifying urban CO2 emissions from space can be approached using different methodologies, including direct plume-based analyses, but combining satellite observations with atmospheric transport models requires the ability to realistically reproduce fine-scale spatial gradients over cities. Using the Grand Paris area as a testbed, we investigate the sensitivity of simulated near-surface CO2 concentrations to urban physics parameterization and horizontal resolution within the WRF-Chem modeling framework coupled to a high-resolution fossil fuel emission inventory. At mesoscale resolution (900 m), a hierarchy of urban representations ranging from simulations without urban physics to multi-layer urban canopy models is evaluated, showing that the Building Energy Model (BEM) provides the most physically consistent simulation of surface energy fluxes, boundary-layer development, and near-surface CO2 variability. Building on this configuration, we compare mesoscale simulations with Large-Eddy Simulation (LES) runs at 300 m and 100 m resolution. Model results are evaluated against dense urban CO2 observations from the high-precision Picarro network, a complementary mid-cost sensor network from ICOS-Cities, and surface sensible and latent heat flux observations from the ICOS ETC Level-2 fluxes data product. An extensive urban observation network including wind lidars and ceilometers from Urbisphere project provides an exceptional constraint for the evaluation of boundary-layer structure and vertical mixing at fine scales. The LES simulations substantially enhance the representation of spatial heterogeneity and localized CO2 enhancements associated with major emission sources, which are smoothed or underestimated at mesoscale resolution. However, increased resolution also amplifies sensitivity to local wind fields and emission inventory uncertainties. These results highlight that both urban physics and model resolution critically shape the ability of transport models to reproduce observed urban CO2 gradients.

How to cite: Rafalimanana, A., Lauvaux, T., Abdallah, C., Chariot, M., Ramonet, M., Doc, J., Laurent, O., Lopez, M., Raznjevic, A., Krol, M., Järvi, L., David, L., Sanchez, O., Christen, A., Looschelders, D., Bignotti, L., Loubet, B., Grimmond, S., and Morrison, W.: Monitoring urban atmospheric CO2 plumes from space: sensitivity to urban physics and scale effects over Paris, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5198, https://doi.org/10.5194/egusphere-egu26-5198, 2026.

EGU26-5426 | ECS | Orals | AS3.38

Quantifying Agricultural Methane Emissions Using Satellite Observations 

Mengyao Liu, Ronald van der A, Michiel van Weele, Elefttherios Ioannidis, Ruoqi Liu, Zichong Chen, and Jieying Ding

Methane (CH₄) is the second most important greenhouse gas after CO₂, and its emissions from the agricultural sector, particularly rice paddies and dairy farms, remain highly uncertain and challenging to quantify. While recent advancements in satellite technology, such as high spatial resolution instruments, have enabled the detection of methane sources from global to facility scales, agricultural emissions still pose challenges. These emissions are typically diffuse and area-like, making them less detectable by targeted satellites like GHGSat and EMIT, which are better suited for isolated point sources such as oil/gas facilities or landfills. Additionally, agricultural emissions exhibit significant spatiotemporal variability driven by climate conditions, water management practices in rice paddies, and differences in farm types.

In the AGATE project of ESA, we apply an improved divergence method to estimate monthly methane emissions using TROPOspheric Monitoring Instrument (TROPOMI) satellite observations at a 0.1° grid resolution. We focus on major agricultural regions, including the Po Valley in Italy, as well as India and Bangladesh, over the period 2019-2022. To better isolate agricultural emissions, we separate area-like sources (e.g., rice paddies) from isolated point sources. The locations of identified big emitters are cross-validated using bottom-up emission inventories and targeted satellite observations (e.g., EMIT, Carbon Mapper) to minimize the influence of non-agricultural sources. Furthermore, to better understand the seasonality of methane emissions, we analyze the correlations between methane emission variations and auxiliary datasets, such as rice paddy maps and ammonia emissions derived from satellites.

How to cite: Liu, M., van der A, R., van Weele, M., Ioannidis, E., Liu, R., Chen, Z., and Ding, J.: Quantifying Agricultural Methane Emissions Using Satellite Observations, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5426, https://doi.org/10.5194/egusphere-egu26-5426, 2026.

EGU26-5912 | ECS | Posters on site | AS3.38

Investigating Germany’s progress in decoupling air pollution emissions from economic activity using satellite-based measurements of NO₂. 

Erika Remy, Rosina Engert, Laurenz Werner, and Michael Bittner

In efforts to mitigate the effects of global climate change several prominent policies and guidelines which emphasize the importance of sustainable growth have been introduced in recent years. Examples include the 2019 European Green Deal, and the subsequent Clean Industrial Deal in 2025. A key aspect of these goals is the reduction of air pollutant emissions, particularly from fossil fuel combustion, without sacrificing economic growth. The Green Deal commits to an EU wide emission reduction of at least 55% by 2030, as compared to 1990 levels. Remote sensing offers many advantages for tracking progress towards reduction of pollutant emissions. In particular, the global coverage allows for analysis of regions which do not have sufficient ground-based measurement networks. This study presents a method of using spectral analysis with tropospheric NO2 column density and the gross domestic product (GDP) to track and compare progress of the German federal states towards decoupling emissions from economic growth. Most studies evaluating economic decoupling focus on CO2, or CO2 equivalences. There is a current lack of studies which investigate other key combustion products. This study focuses on NO2 as a proxy for emissions related to economic activity. NO2 originates primarily from anthropogenic combustion sources, andhas a short tropospheric lifetime, making it suitable to represent localized fossil fuel emissions.  Measurements of NO2 used in this study are obtained from the Ozone Monitoring Instrument (OMI) launched aboard the NASA Aura satellite in 2004. The application of spectral analysis techniques, such as the wavelet analysis, gives additional insight into temporal variability of NO2, to better observe the path of decoupling for each region. Decoupling between GDP and NO2 variability is observed for all regions of Germany in the period between the two most recent global economic recessions (the 2008 financial crisis, and the Covid-19 pandemic). Similar decreasing trends are observed for both the yearly average tropospheric column density and the calculated yearly variability. The variability obtained from the wavelet analysis shows greater sensitivity to changes in NO2 emissions than the absolute tropospheric column density. Further regional differences such as the main economic sectors and types of emission regulations in place are discussed to contextualize the differences present in decoupling processes between the federal states. Overall, NO2 variability is found to be a sensitive and effective indicator for tracking and comparing decoupling progress across different administrative regions.

How to cite: Remy, E., Engert, R., Werner, L., and Bittner, M.: Investigating Germany’s progress in decoupling air pollution emissions from economic activity using satellite-based measurements of NO₂., EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5912, https://doi.org/10.5194/egusphere-egu26-5912, 2026.

EGU26-7798 | ECS | Posters on site | AS3.38

Low latency and high resolution GHG emission estimates to support monitoring and modelling activities in Spain 

Oliver Legarreta, Paula Castesana, Ivan Lombardich, Carles Tena, Carmen Piñero-Megías, Artur Viñas, Johanna Gehlen, Luca Rizza, Carlos Pérez García-Pando, and Marc Guevara Vilardel

Reliable and timely information on greenhouse gas (GHG) emissions is essential for evaluating mitigation policies and supporting data assimilation and verification modelling frameworks. In this contribution, we present the sPanisH EmissioN mOnitoring systeM for grEeNhouse gAses (PHENOMENA), a low-latency GHG modelling framework developed within the RESPIRE-CLIMATE Spanish national project, which received formal endorsement from the WMO-IG3IS initiative.

PHENOMENA provides harmonised daily and high spatial resolution (up to 1 km × 1 km) CO2 and CH4 emissions for the main combustion-related sectors, including electricity generation, manufacturing industry (cement and iron and steel), residential and commercial combustion, road transport, shipping and aviation. The system estimates CO2 and CH4 emissions by combining low latency activity data and fuel- and process-dependent emission factors through bottom-up and downscaling approaches. The data collected and pre-processed includes hourly near-real-time traffic counts from the national road network, hourly electricity production data reported by individual power plants, daily Copernicus ERA5-Land surface temperature, monthly industrial production statistics and AIS (Automatic Identification System) data, among others.

PHENOMENA produces multiple GHG emission products, including high resolution maps of daily emissions per sector, as well as daily summaries of emissions aggregated at different regional levels and for the main Spanish metropolitan regions. The emissions computed with PHENOMENA allows representing the intra-weekly and seasonal variability of GHG emissions as well as changes in their spatial patterns, which can be linked to specific policy, socioeconomic, and weather impacts.

The results produced with PHENOMENA are compared to official GHG emission inventories as well as to other state-of-the-art low latency GHG emission datasets, such as the ones produced by the CAMS Carbon Monitor initiative. Overall, these developments demonstrate the capability of PHENOMENA to deliver consistent, multisector and near-real-time GHG emission estimates, supporting national monitoring, policy evaluation and future verification and data-assimilation efforts.

How to cite: Legarreta, O., Castesana, P., Lombardich, I., Tena, C., Piñero-Megías, C., Viñas, A., Gehlen, J., Rizza, L., Pérez García-Pando, C., and Guevara Vilardel, M.: Low latency and high resolution GHG emission estimates to support monitoring and modelling activities in Spain, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7798, https://doi.org/10.5194/egusphere-egu26-7798, 2026.

EGU26-7927 | Orals | AS3.38

Using point source imaging satellite observations to guide landfill methane model improvements at the national and sub-national scale 

Tia Scarpelli, Daniel Cusworth, Jinsol Kim, Kelly O'Neill, Riley Duren, and Katherine Howell

As national and sub-national governments, companies, and communities plan methane mitigation action, there is a need for robust emissions tracking systems, especially for major sectors like waste where countries have made commitments to reduce emissions. Landfills are a major source of methane emissions in many jurisdictions spread across the world, so there is a need in the waste sector for monitoring frameworks that are applicable at scale but also provide facility-level insights to guide decision making. 

 

Given the complexity of landfill emissions both in terms of variability and underlying causes, models are a common tool used for planning and tracking landfill methane mitigation, but past studies show potential biases in models and inventories compared to observations. In this work, we bring together both process-level insights as provided in bottom-up models and our top-down observations from the Tanager-1 satellite by (1) improving the accuracy and consistency of satellite-derived annual average emission rates and (2) developing methodologies for reconciling the two unique datasets. The goal of this work is to use satellite methane observations to identify improved bottom-up model parameters, focusing on the modeling frameworks used by national and sub-national jurisdictions.

 

As a point source imaging satellite, Tanager-1 is well suited for tracking emissions at landfills as it provides facility-scale methane emissions data, but existing algorithms and workflows for creating the emissions data have been primarily validated based on controlled release experiments which mimic environments more similar to the oil and gas sector than landfills. We identify methods that are robust and best suited to landfills by performing sensitivity tests for our quantification methods, testing algorithms and parameters, and identifying causes of bias unique to landfill environments (e.g., albedo, topography). The next step is translating our Tanager-1 observations to annual averages. We present a new methodology for temporally averaging satellite observations that accounts for null detects through scene-specific probability of detection limits. Finally, we compare our annual average satellite-based emission estimates to bottom-up models typically used by jurisdictions for official reporting (e.g., IPCC, LandGEM, US GHGRP), focusing on select countries where there is sufficient spatiotemporal coverage with Tanager-1. We use statistical methods to adjust parameters in the bottom-up models to reconcile the model estimates with observed emissions, allowing region-specific model parameter adjustments to account for potential climatic and meteorological factors. Finally, we discuss the implications of our initial results in terms of improvements to official national reporting and compare to inverse modeling results.

How to cite: Scarpelli, T., Cusworth, D., Kim, J., O'Neill, K., Duren, R., and Howell, K.: Using point source imaging satellite observations to guide landfill methane model improvements at the national and sub-national scale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7927, https://doi.org/10.5194/egusphere-egu26-7927, 2026.

EGU26-8459 | Posters on site | AS3.38

Validating environmental reporting of carbon emissions 

Lee Stokes, Aleksandra Przydrozna, and Valerie Livina

ESG (Environmental, Social, Governance) reporting is essential for industry as it helps secure investment for companies’ development. While Scope 1 are direct emissions and Scope 2 are indirect emissions, most of the industrial players report Scope 2 emissions from the use of energy (electricity and gas): these are carbon emissions that are emitted in the power station that uses fossil fuels (oil, coal, gas, biomass, etc.), see [1].

Conventional way to report company’s carbon emissions of Scope 2 is to obtain electrical meter readings and multiply them by the average carbon intensity of the electric grid that supplies electricity. In the UK, such carbon factors were previously published (annually) by the Department for Environment, Food, and Rural Affairs (Defra), then more recently by the Department for Energy Security and Net Zero (DESNZ). These average annual factors are approximate, and actual fuel mix of the electrical grid varies within a few minutes, depending on the operating power generators.

In some cases, the annual carbon intensity may underestimate the actual intensity of the grid. This usually happens in Europe in winter, when a large number of gas-fuelled generators are active to provide sufficient heating, and at the same time wind conditions are placid, providing little of renewable energy. In other cases, when there is lots of wind-generated energy and less gas-generated energy (for example, on a windy summer day), the average carbon factor may overestimate actual carbon intensity of the grid.

In several case studies, we demonstrate that such discrepancies may reach 10-15% of the total carbon emissions, as they are presented in quarterly or annual ESG reports. The results suggest that the current way of reporting carbon emissions should be revised, so that actual state of the dynamical energy grid would be taken into account for improvement of ESG reporting. Subsequently, this will impact their ESG standing and potential investment, which is crucial for European business as well as for the correct accounting of the impact of European carbon emissions [2].

References

[1] Livina et al, International Journal of Metrology and Quality Engineering, in revision.

[2] Livina et al, in preparation.

How to cite: Stokes, L., Przydrozna, A., and Livina, V.: Validating environmental reporting of carbon emissions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8459, https://doi.org/10.5194/egusphere-egu26-8459, 2026.

Reducing methane (CH4​) emissions through environmentally friendly agriculture, such as Alternate Wetting and Drying (AWD), is a critical strategy for climate change mitigation in rice production. To effectively implement and evaluate these mitigation measures, it is essential to monitor agricultural practices and environmental variables at a high spatial resolution. This study develops a standardized data-processing protocol, which leverages Google Earth Engine (GEE) to generate high-resolution remote sensing features necessary for quantifying CH4​ emissions.

The protocol integrates multi-sensor satellite data to capture the spatio-temporal dynamics of sustainable rice farming. Central to this protocol is the use of Sentinel-1 Synthetic Aperture Radar (SAR) data to classify water management regimes, specifically distinguishing between continuous flooding (CF) and AWD at the pixel level. Additionally, Sentinel-2 optical imagery is processed to extract key vegetation indices (e.g., NDVI, GRVI) to monitor crop growth. To address environmental factors, coarse-resolution soil moisture data from SMAP is downscaled to resolution by incorporating Sentinel-2 and Digital Elevation Model (DEM) data.

By synthesizing these multi-sensor inputs, the protocol provides the necessary foundation for mapping methane emission hotspots and assessing the impact of environmentally friendly management practices. This high-resolution approach supports the design of region-specific mitigation strategies and the advancement of climate-smart agriculture.

As for future research plans, we will apply the constructed model with the field-measured validation data to the extensive rice paddies in southern Ibaraki Prefecture in Japan to estimate methane emissions on a pixel-by-pixel basis and create hotspot maps. This enables the upscaling of a single-point observation model to a broader area while reflecting regional characteristics. This methodology is expected to serve as a powerful tool for examining highly effective methane reduction measures (such as utilization under the J-Credit system) based on each region's agricultural practices and environmental conditions.

How to cite: Shoyama, K., Hirai, C., and Den, H.: Monitoring Environmentally Friendly Agriculture for Methane Emission Reduction: A High-Resolution Multi-Sensor Remote Sensing Protocol on Google Earth Engine, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8591, https://doi.org/10.5194/egusphere-egu26-8591, 2026.

EGU26-9177 | Posters on site | AS3.38

Transport model error in inverse modelling: Developments within the ITMS project 

Christoph Gerbig, Michal Galkowski, Frank-Thomas Koch, Lena Danyeli, Fabian Maier, Saqr Munassar, Yang Xu, and Christian Rödenbeck

Inverse modelling of CO2 and CH4 using atmospheric in-situ data relies on simulations of atmospheric transport that arederived from models used in numerical weather prediction. The relevant time scales for inversions range from hours to decades, which is far beyond the time scales of a few weeks for which NWP models are designed. The strong diurnal and seasonal variations in surface to atmosphere fluxes of CO2 covary with atmospheric mixing in the boundary layer, as both are solar radiation driven. This way slight seasonal or diurnal biases in the representation of mixing can be amplified. In addition, different atmospheric models show differences in vertical mixing through turbulent mixing and through moist convection, and thus in the representation of vertical gradients in tracers, which results strong differences in flux estimates from inverse modelling. These facts have been known since several decades by now, but progress in addressing these issues has been slow. Within the atmospheric network of ICOS (Integrated Carbon Observation System) additional meteorological observations are available that provide information on atmospheric mixing heights. Also, IAGOS (In-service Aircraft for a Global Observing System) provides information on vertical gradients which can be related to mixing through turbulence and convection.

ITMS, the Integrated Greenhouse gas Monitoring system for Germany, is implemented in multiple development phases: a first phase with the development of a demonstrator system, followed by the second phase, the development of a first-generation system, and a third and last phase, the transfer to operations. With each phase lasting about four years, the project provides a medium-term framework that allows also addressing some of the longer lasting problems such as transport uncertainty. Within ITMS the CarboScope Regional inversion system (CSR) is used as a reference system for CO2 and CH4 inversions, but also as a testbed for model developments. The presentation will provide an overview of recent results obtained within ITMS. This includes evaluating vertical mixing by using additional meteorological profile data or mixing height information, using additional tracers in inversions such as Radon, and confronting vertical profiles from airborne observations with model equivalents. 

How to cite: Gerbig, C., Galkowski, M., Koch, F.-T., Danyeli, L., Maier, F., Munassar, S., Xu, Y., and Rödenbeck, C.: Transport model error in inverse modelling: Developments within the ITMS project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9177, https://doi.org/10.5194/egusphere-egu26-9177, 2026.

EGU26-9574 | ECS | Orals | AS3.38

A global coal mine methane tracker to highlight inventory gaps and target mitigation 

Rebekah Horner, Sabina Assan, and Adomas Liepa

Methane (CH4) is a key short-lived climate forcer, yet robust monitoring of its anthropogenic sources remains limited by inconsistent national reporting and incomplete inventories, especially from coal mining. Global anthropogenic CH4 emissions are about 369 million tonnes per year, of which coal mine methane (CMM) contributes roughly 40 million tonnes per year, which is comparable to emissions from the gas sector. In 2023 only 15% of coal production reported annual CMM emissions in national greenhouse gas inventories and this limits the scientific basis for monitoring and verification of progress towards the Global Methane Pledge and the Paris Climate Agreement.

We present Ember’s Coal Mine Methane Data Tracker as a new open, global, evidence based dataset for understanding CMM emissions, reporting quality and methane targets. The Data Tracker compiles and harmonises national greenhouse gas inventory submissions to the United Nations Framework Convention on Climate Change (UNFCCC). It integrates these data with historic coal production statistics from the US Energy Information Administration (EIA), International Energy Agency (IEA) coal production forecasts and independent emission estimates (IEA Methane Tracker, Global Energy Monitor (GEM) Global Coal Mine Tracker).

To reconstruct national emissions from 1990 onwards, we calculate country and year specific CH4 emission intensities wherever both reported emissions and coal production exist. Emission intensity is defined as CH4 emissions (in kilotonnes) per million tonnes of coal produced. This approach also enables consistent comparison of reported emissions across countries and over time.

We fill gaps in the intensity time series using values from neighbouring years so that each country has a continuous record. We then multiply these completed intensity series by observed production to estimate unreported emissions. Ember’s gap filled series indicates that global active CMM emissions exceeded 34 million tonnes in 2023, whereas official UNFCCC inventories reported only 4.62 million tonnes, less than 14% of the inferred total. For 2024, the latest compilation of submissions implies 34.5 million tonnes of reported CMM, with underreporting of up to 21.2 million tonnes when compared with independent datasets.

We introduce a quantitative confidence score from 0 to 6 for each country’s reported CMM emissions, combining recency of UNFCCC reporting, consistency with independent estimates from both top down and bottom up approaches, and methodological robustness. Applied to major producers, this score shows that most large coal producing countries fall in the low-to-moderate confidence range, with only a small number, such as Poland (score 5), achieving higher confidence in their reported CMM inventories. 

By providing a transparent, harmonised framework for CMM monitoring, we demonstrate that systematic underreporting pervades national inventories. This gap is driven by widespread reliance on low tier IPCC methods, with 86% of reported CMM emissions relying on emission factors rather than direct measurement. Our quantitative confidence score (ranging from 0 to 6) highlights this reliance, showing that low scoring countries correlate directly with significant underestimation. This evidence necessitates the need for transparent, measurement based Monitoring, Reporting and Verification (MRV) frameworks to establish the rigorous CH4 accounting required by global climate commitments.

How to cite: Horner, R., Assan, S., and Liepa, A.: A global coal mine methane tracker to highlight inventory gaps and target mitigation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9574, https://doi.org/10.5194/egusphere-egu26-9574, 2026.

EGU26-10112 | ECS | Posters on site | AS3.38

Urban greenhouse gas monitoring across the Barcelona Metropolitan Area 

Vanessa Monteiro, Gara Villalba Mendez, Qing Luo, and Roger Curcoll Masanes

An urban greenhouse gas (GHG) monitoring network has been established in the Barcelona Metropolitan Area to support the evaluation of GHG mitigation strategies. The network currently consists of five measurement sites equipped with high-precision Picarro analysers providing continuous observations of carbon dioxide (CO2) and methane (CH4). These measurements, in combination with atmospheric modelling will be used to investigate spatial and temporal variability in urban GHG concentrations.

The five sites (Fabra, ICM, ICTA, IDAEA, and UPC-Agropolis) were strategically selected to represent a range of urban and peri-urban environments, including a natural forest, an urban coastal site, a traffic-influenced highway location on the outskirts of the city, an urban park embedded within a densely built area, and a peri-urban agricultural region. This configuration enables the assessment of how different landuse types and emission sources influence observed GHG mole fractions across the metropolitan area.

Hourly averaged CO2 mole fractions show pronounced differences between sites. Lower values are observed at the forested Fabra site, while the ICTA site, located near a major highway, exhibits the highest mole fractions and the largest variability. These spatial contrasts are consistent with results from previous multi-site measurement campaigns in Barcelona, which indicated that densely urbanized, impermeable landscapes are associated with enhanced CO2 concentrations compared to greener areas, particularly during morning hours dominated by traffic emissions.

Maintaining a continuous urban monitoring network is essential for capturing both spatial and temporal variability in GHG concentrations and for improving our understanding of urban atmospheric processes. Such observations are also critical for constraining and validating atmospheric models and for quantifying changes in emissions over time. Here, we present recent observations from the Barcelona Metropolitan Area GHG network and illustrate their application to the study of greenhouse gas variability in complex urban environments.

How to cite: Monteiro, V., Villalba Mendez, G., Luo, Q., and Curcoll Masanes, R.: Urban greenhouse gas monitoring across the Barcelona Metropolitan Area, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10112, https://doi.org/10.5194/egusphere-egu26-10112, 2026.

EGU26-10768 | ECS | Posters on site | AS3.38

Forward modelling of SF6 with ICON-ART 

Maya Harms, Katharina Meixner, Tanja Schuck, Thomas Wagenhäuser, Sascha Alber, Kieran Stanley, Andreas Engel, Valentin Bruch, Thomas Rösch, Martin Steil, and Andrea Kaiser-Weiss

Sulfur hexafluoride (SF6) is a highly potent greenhouse gas (GHG). Despite its high global warming potential (GWP), it continues to be produced and used in Germany. The reported emission estimates can be used to calculate expected concentrations at measurements sites. Within the PARIS (Process Attribution of Regional Emissions) project we used the operational numerical weather prediction model ICON (ICOsahedral Nonhydrostatic) and its extension module for aerosol and trace gases (ART) as an Eulerian forward model to calculate the expected mixing concentrations response of Germany's largest point source of SF6. We compared the modelled concentration peaks that occur when the modelled plume crosses the measurement site of the Taunus observatory (TOB) with the respective observed signals (requiring background subtraction). The 4-year period of 2020-2023 was covered, and the uncertainty of the meteorological transport was estimated using a 20-member ensemble in our limited area model for Europe, which was run with a horizontal grid resolution of 6.5 km and 74 vertical levels.The model predicts well when peaks are measured but weWe found that most observed peaks at TOB are considerably higher than in the model, suggesting that prior emissions estimates were too low. 
This indicates that the independent, observation-based emission estimate of our ICON-ART based system is in the range of double-digit tons, which is considerably higher than the self-reported SF6 emission estimate for this point source, also if the model uncertainties are taken into account. 

How to cite: Harms, M., Meixner, K., Schuck, T., Wagenhäuser, T., Alber, S., Stanley, K., Engel, A., Bruch, V., Rösch, T., Steil, M., and Kaiser-Weiss, A.: Forward modelling of SF6 with ICON-ART, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10768, https://doi.org/10.5194/egusphere-egu26-10768, 2026.

EGU26-11447 | ECS | Posters on site | AS3.38

Satellite-Based Estimation of Nitrous Oxide Concentration and Emission in a Large Estuary 

Wenjie Fan and Zhihao Xu

Estuaries are nitrous oxide (N2O) emission hotspots and play an important role in the global N2O budget. However, the large spatiotemporal variability of emission in complex estuary environments is challenging for large-scale monitoring and budget quantification. This study retrieved water environmental variables associated with N2O cycling based on satellite imagery and developed a machine learning model for N2O concentration estimations. The model was adopted in China’s Pearl River Estuary to assess spatiotemporal N2O dynamics as well as annual total diffusive emissions between 2003 and 2022. Results showed significant variability in spatiotemporal N2O concentrations and emissions. The annual total diffusive emission ranged from 0.76 to 1.09 Gg (0.95 Gg average) over the past two decades. Additionally, results showed significant seasonal variability with the highest contribution during spring (31 ± 3%) and lowest contribution during autumn (21 ± 1%). Meanwhile, emissions peaked at river outlets and decreased in an outward direction. Spatial hotspots contributed 43% of the total emission while covering 20% of the total area. Finally, SHapley Additive exPlanations (SHAP) was adopted, which showed that temperature and salinity, followed by dissolved inorganic nitrogen, were key input features influencing estuarine N2O estimations. This study demonstrates the potential of remote sensing for the estimation of estuarine emission estimations.

How to cite: Fan, W. and Xu, Z.: Satellite-Based Estimation of Nitrous Oxide Concentration and Emission in a Large Estuary, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11447, https://doi.org/10.5194/egusphere-egu26-11447, 2026.

EGU26-11719 | ECS | Posters on site | AS3.38

Using atmospheric observations to identify point sources of halogenated trace gases 

Katharina Meixner, Dominique Rust, Tanja J. Schuck, Thomas Wagenhäuser, Fides Gad, Cedric Couret, Armin Jordan, Martin Vojta, Andreas Stohl, and Andreas Engel and the PARIS project

Measurement-based emission estimates derived from atmospheric observations provide an independent and important approach for identifying emission sources, quantifying emissions and verifying reported inventories. This is particularly relevant for halogenated gases, which due to their role as ozone depleting substances and potent greenhouse gases are regulated under various international and national frameworks. Here, we present two studies highlighting the urgency and the challenges of the measurement-based emission estimates of sulfur hexafluoride (SF6) and fluoroform (HFC-23) with a particular focus on the influence of point sources.

SF6 and HFC-23 are two of the most potent greenhouse gases with a GWP100 of approximately 24,000 and 14,700, respectively. Previous studies consistently showed a dominant emission source in southern Germany contributing to a large share of European SF6 emissions. Meixner et al., 2025 analysed emission estimates based on 22 European measurement sites revealing an underestimated SF6 emission point source in southern Germany in contrast to the national inventory reports.

Recent studies highlighted major challenges in quantifying HFC-23 emissions (Adam et al., 2024; Rust et al., 2024). We investigate the effects of intermittency in emissions and explore different possibilities based on a priori assumptions about specific emission sources. Forward calculations from these potential emission sources are used to derive expected time series at observational sites. These are compared to observations from different European stations situated in the regions influenced by the potential point sources. We present different approaches based on European atmospheric measurements combined with multiple model approaches, including ICON-ART, FLEXPART and NAME.

Adam, B., Western, L.M., Mühle, J., Choi, H., Krummel, P.B., O’Doherty, S., Young, D., Stanley, K.M., Fraser, P.J., Harth, C.M., Salameh, P.K., Weiss, R.F., Prinn, R.G., Kim, J., Park, H., Park, S., Rigby, M., 2024. Emissions of HFC-23 do not reflect commitments made under the Kigali Amendment. Commun. Earth Environ. 5, 783. https://doi.org/10.1038/s43247-024-01946-y

Meixner, K., Wagenhäuser, T., Schuck, T.J., Alber, S., Manning, A.J., Redington, A.L., Stanley, K.M., O’Doherty, S., Young, D., Pitt, J., Wenger, A., Frumau, A., Stavert, A.R., Rennick, C., Vollmer, M.K., Maione, M., Arduini, J., Lunder, C.R., Couret, C., Jordan, A., Gutiérrez, X.G., Kubistin, D., Müller-Williams, J., Lindauer, M., Vojta, M., Stohl, A., Engel, A., 2025. Characterization of German SF6 Emissions. ACS EST Air 2, 2889–2899. https://doi.org/10.1021/acsestair.5c00234

Rust, D., Vollmer, M.K., Henne, S., Frumau, A., van den Bulk, P., Hensen, A., Stanley, K.M., Zenobi, R., Emmenegger, L., Reimann, S., 2024. Effective realization of abatement measures can reduce HFC-23 emissions. Nature 633, 96–100. https://doi.org/10.1038/s41586-024-07833-y

How to cite: Meixner, K., Rust, D., Schuck, T. J., Wagenhäuser, T., Gad, F., Couret, C., Jordan, A., Vojta, M., Stohl, A., and Engel, A. and the PARIS project: Using atmospheric observations to identify point sources of halogenated trace gases, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11719, https://doi.org/10.5194/egusphere-egu26-11719, 2026.

EGU26-11963 | Posters on site | AS3.38

 Bridging Science and National GHG Inventories: Insights from the PARIS Project – Process Attribution of Regional Emissions 

Sylvia Walter, Alistair Manning, Thomas Röckmann, and Anita Ganesan and the PARIS Team

Strengthening the link between scientific research and official greenhouse gas (GHG) reporting is an important step under the Paris Agreement’s Enhanced Transparency Framework. The PARIS Project, funded by Horizon Europe, is working with eight European countries to develop practical tools for this purpose.

A central innovation of PARIS is the development of draft annexes to National Inventory Documents (NIDs). These annexes provide a structured and transparent interface between official bottom-up inventories and top-down atmospheric estimates. They do not alter formal reporting rules; instead, they document how independent scientific assessments compare with inventory estimates, identify consistencies and discrepancies, and highlight where further investigation or methodological development is warranted. In this way, the annexes enable inventory compilers, policymakers, and scientists to interpret atmospheric results within the legal and institutional framework of national reporting.

The annexes are underpinned by major advances in PARIS observation and modelling capacity. Expanded and harmonised networks for CH₄, N₂O, F-gases, and aerosols, together with multi-model inverse systems and common data standards publicly available on the ICOS Carbon Portal, provide robust, traceable estimates of regional emissions and their sectoral drivers. These scientific outputs are synthesised in the annexes in a form that is directly usable by inventory agencies.

Through close engagement with national inventory teams in the UK, Switzerland, Germany, Ireland and other focus countries, PARIS has co-developed annex templates and begun populating them with results from multiple inversion systems. This process reduces barriers between the research and inventory communities and supports routine, transparent comparison of bottom-up and top-down estimates.

The poster will present the main outcomes of the PARIS project, demonstrating how the outcomes advance and embed atmospheric science in national GHG reporting to strengthen confidence in emission estimates, improve process attribution of regional emissions, and ultimately support more effective climate policy under the Paris Agreement.

How to cite: Walter, S., Manning, A., Röckmann, T., and Ganesan, A. and the PARIS Team:  Bridging Science and National GHG Inventories: Insights from the PARIS Project – Process Attribution of Regional Emissions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11963, https://doi.org/10.5194/egusphere-egu26-11963, 2026.

EGU26-12319 | ECS | Orals | AS3.38

The use of CLMS products for improving the spatialization of greenhouse gases emissions from LULUCF and agriculture sectors  

Giulia Cecili, Paolo De Fioravante, Guido Pellis, Marina Vitullo, and Angela Fiore

The Land Use, Land-Use Change, and Forestry (LULUCF) and agriculture sectors are increasingly central to global climate policy. They play a crucial role in climate mitigation strategies, as land acts as a carbon sink that needs to be enhanced and as a source of greenhouse gas (GHG) emissions that must be reduced. In the European context, the LULUCF Regulation (EU 2018/841), revised in 2023, aims for 310 Mt CO2eq net removals by 2030 and requires spatially explicit land-use representations to monitor land dynamics and assess policy impacts.

Within the Horizon project AVENGERS (Attributing and Verifying European and National Greenhouse Gas and Aerosol Emissions and Reconciliation with Statistical Bottom-up Estimates), a methodology was developed to generate an IPCC-compliant land-use map by integrating multiple Copernicus Land Monitoring Service (CLMS) products. In national GHG inventories, the operational use of spatial explicit data is often limited due to restricted temporal coverage, inconsistencies with national statistics, and challenges in interpreting mixed classes and land-use/land cover definitions. This methodology provides a transparent approach to reconcile inventory data with high-resolution spatial datasets.

The approach combines the CLC Plus Backbone geometry with CORINE Land Cover (CLC) and ancillary CLMS datasets, including the High-Resolution Layer Crop Types and Priority Areas monitoring products (e.g., Coastal Zones, Riparian Zones, and Protected areas). Multiple layers were integrated using overlay techniques and priority rules, resulting in an harmonized map at 10-m spatial resolution. CLC attributes were aggregated to IPCC land use categories, allowing direct comparison between mapped areas and inventory surfaces.

Preliminary validation involved cross-checks with national land-use activity data to ensure reliability of mapped areas across LULUCF categories. The resulting maps enable the spatialization of inventory-based LULUCF and agriculture emissions, producing gridded emission datasets based on improved spatially explicit land-use information. These datasets are suitable for use as input (priors) in atmospheric inversion modelling, a top-down emissions estimation method supporting policy evaluation.

The methodology is designed to be replicable across all European countries covered by CLMS data and to be updated approximately every 2–3 years, in line with the regular update cycle of CLMS products. The methodological framework is modular and flexible, based on a spatial data storage and management scheme developed by ISPRA, which allows the integration of additional datasets and adaptation to different territorial contexts. The approach was applied and tested in three national case studies for the year 2018—Italy, Sweden, and the Netherlands—with specific adaptations introduced to account for distinct territorial characteristics. This first implementation represents a promising step and provides a solid foundation for further refinements and future developments, supporting the production of high-resolution land-use maps helpful for national inventory agencies and inversion modelling experts.

How to cite: Cecili, G., De Fioravante, P., Pellis, G., Vitullo, M., and Fiore, A.: The use of CLMS products for improving the spatialization of greenhouse gases emissions from LULUCF and agriculture sectors , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12319, https://doi.org/10.5194/egusphere-egu26-12319, 2026.

EGU26-12745 | ECS | Posters on site | AS3.38

Impact of Local-Scale Effects in Methane (CH₄) Inversions on Model-Observation Discrepancies 

Elena Zwerschke, Frank-Thomas Koch, Christoph Gerbig, Jennifer Mueller-Williams, Matthias Lindauer, Frank Keppler, and Dagmar Kubistin

Accurate estimates of greenhouse gas emissions are critical for determining the effectiveness of mitigation strategies under the Paris Agreement. These estimates are commonly derived by atmospheric inversion frameworks, which combine atmospheric transport models with in situ observations to obtain greenhouse gas fluxes. However, regional inversions are often challenged by local-scale signals in atmospheric measurements, that are insufficiently represented by the models. If not properly accounted for, these can introduce biases in inverse flux estimates undermining the reliability of emission estimates.

To address this limitation, observational data has typically been filtered for local influences before being used in inversion simulations, based on assumptions such as stable boundary conditions or wind speed. To make full use of the available dataset, we implemented an observation-dependent model-data uncertainty in the inversion optimisation process, allowing local signals to be explicitly considered. This approach has been applied to CH4 inversions over Europe using the mesoscale Jena CarboScope-Regional (CSR) system at 0.25° × 0.25° resolution.

To determine the time varying model-data uncertainty based on the local influence signal, a leave-one-out cross validation was performed for ground based in situ data of 47 atmospheric stations, excluding one station per inversion simulation. By determining the difference between modelled and observed concentrations, a model-data mismatch was estimated across station categories defined by surrounding land type. These estimates were then combined with local signal features, resulting from low wind speeds, atmospheric stability, and concentration spikes using a multivariate regression. The derived model-data mismatch function was applied to adjust the data weighting in the inversion enabling the inclusion of the observational dataset without discarding any measurements.

In this presentation, we demonstrate the potential of this novel approach to improve the robustness of regional CH4 inversions and to reduce the bias from local-scale signals.

How to cite: Zwerschke, E., Koch, F.-T., Gerbig, C., Mueller-Williams, J., Lindauer, M., Keppler, F., and Kubistin, D.: Impact of Local-Scale Effects in Methane (CH₄) Inversions on Model-Observation Discrepancies, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12745, https://doi.org/10.5194/egusphere-egu26-12745, 2026.

EGU26-12776 | ECS | Posters on site | AS3.38

Quantifying European SF6 emissions (2005-2021) using a large ensemble of atmospheric inversions 

Martin Vojta, Andreas Plach, Rona L. Thompson, Pallav Purohit, Kieran Stanley, Simon O'Doherty, Dickon Young, Joe Pitt, Jgor Arduini, Xin Lan, and Andreas Stohl

Sulfur hexafluoride (SF₆) is an extremely potent (GWP100 = 24,300) and long-lived greenhouse gas whose atmospheric concentrations continue to rise due to anthropogenic emissions. Europe represents a particularly relevant test case for investigating SF₆ emissions, as successive EU F-gas regulations over the past two decades have aimed to substantially reduce emissions. A key question is whether these regulatory measures are reflected in observed emission trends and whether reported national inventories are consistent with observation-based estimates.

 In this study, we quantify European SF₆ emissions for the period 2005–2021 using a large ensemble of atmospheric inversions with a strong focus on uncertainty characterization. Uncertainties are assessed using an extensive set of sensitivity tests in which key inversion parameters are systematically varied, while final uncertainties are quantified via a Monte Carlo ensemble that randomly samples combinations of these parameters. This allows us to identify the main sources of uncertainty and to evaluate the robustness of inferred emission trends.

Our analysis focuses on countries with relatively dense observational coverage - the United Kingdom, Germany, France, and Italy - while also examining aggregated emissions for the EU-27.  The inversion results reveal declining SF₆ emissions in all studied regions except Italy, broadly consistent with the timing of EU F-gas regulations (842/2006, 517/2014). In several countries, inferred emissions exceed reported national inventories, although the agreement generally improves in more recent years. At the EU-27 scale, emissions exhibit a pronounced decline between 2017 and 2018, coinciding with a marked reduction in emissions from southwestern Germany, suggesting regional actions were taken as the 2014 regulation took effect.

Our sensitivity tests highlight the crucial role of dense and sustained atmospheric monitoring networks for robust inversion-based emission estimates. In particular, expansions of the UK observing system in 2012 and 2014 lead to significant reductions in emission uncertainties, demonstrating the importance of comprehensive observational networks in refining emission estimates.

How to cite: Vojta, M., Plach, A., Thompson, R. L., Purohit, P., Stanley, K., O'Doherty, S., Young, D., Pitt, J., Arduini, J., Lan, X., and Stohl, A.: Quantifying European SF6 emissions (2005-2021) using a large ensemble of atmospheric inversions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12776, https://doi.org/10.5194/egusphere-egu26-12776, 2026.

EGU26-14303 | ECS | Orals | AS3.38

Urban Atmospheric Monitoring and Modeling System (Urban-AMMS): A Top-Down Approach to Investigate Sources and Variability of an Inert Tracer in the Washington, DC, and Baltimore, MD, Metropolitan Area 

Miguel Cahuich-Lopez, Christopher Loughner, Fong Ngan, Anna Karion, Lei Hu, Israel Lopez-Coto, Kimberly Mueller, Julia Marrs, John Miller, Brian McDonald, Colin Harkins, Congmeng Lyu, Meng Li, Kevin Gurney, Sonny Zinn, Xinrong Ren, Mark Cohen, Howard Diamond, Ariel Stein, and James Whetstone

Accurate quantification of the sources and sinks of long-lived air pollutants is fundamental for effective emissions management, particularly in urban areas where emissions are generally more intense. Stakeholders commonly use so-called bottom-up methods to estimate emissions for urban areas. This type of emission accounting is typically carried out for annual totals, often with a latency of one or more years. Alternative methods that provide estimates with higher temporal resolution and lower latency could be helpful for stakeholders seeking targeted strategies to reduce emissions. A top-down urban emissions estimation system for the Washington, DC, and Baltimore, MD, metropolitan area, called the Urban Atmospheric Monitoring and Modeling System (Urban-AMMS), is being developed to provide accurate, up-to-date urban emissions data. Urban-AMMS has several components, including tower-based, aircraft, and mobile van measurements platforms, whose data are assimilated by the CarbonTracker-Lagrange analytical inverse model; an ensemble of HYSPLIT backward dispersion simulations driven by in-house high-resolution WRF simulations (spatial resolution of 1 km) enhanced with urban meteorological observations; biospheric models; and bottom-up inventories used for a prior estimate of emissions in the domain. The inversion system is tailored to account for the underlying variability in urban fluxes of an inert tracer (CO2) by solving for hourly fluxes and incorporating explicit spatiotemporal covariance of prior errors, as well as high-resolution source-receptor sensitivities estimated by WRF-HYSPLIT. Here, we present an overview of Urban-AMMS, including initial results and sensitivity analyses to investigate the effects of prior spatial aggregation, background handling, and the temporal covariance of prior errors. Numerical experiments show improvements in estimates of urban surface fluxes at both the city and grid cell scales. Still, the reliability of inverse fluxes depends on prior uncertainty, as observed in previous studies. These findings provide critical insights for the inverse estimation of long-lived air pollutants in complex urban environments.

How to cite: Cahuich-Lopez, M., Loughner, C., Ngan, F., Karion, A., Hu, L., Lopez-Coto, I., Mueller, K., Marrs, J., Miller, J., McDonald, B., Harkins, C., Lyu, C., Li, M., Gurney, K., Zinn, S., Ren, X., Cohen, M., Diamond, H., Stein, A., and Whetstone, J.: Urban Atmospheric Monitoring and Modeling System (Urban-AMMS): A Top-Down Approach to Investigate Sources and Variability of an Inert Tracer in the Washington, DC, and Baltimore, MD, Metropolitan Area, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14303, https://doi.org/10.5194/egusphere-egu26-14303, 2026.

EGU26-14957 | Orals | AS3.38

Quantifying N₂O Flux over the EU27+3 Region Using CIF-CHIMERE Model for 2005–2023 

Tianqi Shi, Antoine Berchet, and Philippe Ciais

Nitrous oxide (N₂O) is the third most important long-lived greenhouse gas after CO₂ and CH₄, yet large uncertainties remain in its regional emission estimates. In this study, we apply the regional inverse modeling system CIF-CHIMERE to quantify N₂O surface fluxes over the EU27+3 region (European Union, United Kingdom, Norway, and Switzerland) for the period 2005–2023, providing a long-term and high spatiotemporal resolution assessment of N2O fluxes. The inversion is primarily constrained by in situ atmospheric N₂O measurements from the ICOS (Integrated Carbon Observation System) ground-based station network across Europe, and uses the CIF-CHIMERE transport model coupled with a four-dimensional variational (4D-Var) data assimilation framework to estimate posterior N2O fluxes. For 2005–2023, inversions are conducted at a spatial resolution of 0.5° × 0.5°, while for 2018–2023 the resolution is refined to 0.2° × 0.2°. In both configurations, hourly surface fluxes are estimated, enabling analysis of diurnal, seasonal, and interannual variability. The inversions significantly improve the representation of localized emission patterns and short-term flux dynamics. Overall, the results provide a top-down dataset for evaluating bottom-up inventories and for improving the understanding of regional and temporal variability in N₂O emissions across EU27+3.

How to cite: Shi, T., Berchet, A., and Ciais, P.: Quantifying N₂O Flux over the EU27+3 Region Using CIF-CHIMERE Model for 2005–2023, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14957, https://doi.org/10.5194/egusphere-egu26-14957, 2026.

EGU26-15692 | ECS | Posters on site | AS3.38

CH4 emissions in Vietnamese Rice Agriculture: Benchmarking process-based model approaches (Tier 3) against Tier 1/2 Estimates 

Chien Nguyen, David Kraus, Tanh Nguyen, Reiner Wassmann, Klaus Butterbach-Bahl, Thi Bach Thuong Vo, Van Trinh Mai, Thi Phuong Loan Bui, and Ralf Kiese

Rice cultivation is the largest source of methane (CH4) emissions in Vietnam’s agricultural sector, making accurate quantification of these emissions critical for national GHG inventories and the design of mitigation policies. Currently, for UNFCCC GHG reporting, Vietnam primarily employs IPCC Tier 2 approaches using national emission factors combined with Tier 1 scaling factors. With the implementation of large-scale mitigation projects and Vietnam’s ambition to achieve Net Zero by 2050, Methane Global Pledge commitment by 2030, and joining international carbon markets, there is an urgent need to transition towards higher-tier methodologies. However, also process-based model (Tier 3) outputs are associated with uncertainty, which needs to be benchmarked first with established Tier 1 and 2 emission estimates.

In this study, CH4 emission data from 13 Vietnamese field experiments are split into two groups—one with comprehensive management information (sufficient data) and one with sparse information (limited data)—to test IPCC Tier methods under different activity data conditions. Furthermore, for Tier 3, an inter-comparison is conducted between two biogeochemical models, DNDC and LandscapeDNDC. The evaluation focuses on the performance in estimating rice yields, seasonal CH4 emissions, and daily flux dynamics, while also analyzing the impact of different model parameterization and simulation setups.

Our evaluation shows that Tier 1 significantly underestimates CH4 emissions, whereas Tier 2 provides a substantial improvement and remains robust across varying soil and management conditions. In contrast, Tier 3 outperforms Tier 2 only when comprehensive management data is available, reflecting its distinctive capacity to represent daily emission dynamics and management-driven peaks.  Consequently, while Tier 2 remains a practical choice for national inventories, Tier 3 is essential for high-resolution mitigation assessments, particularly for large-scale emission reduction evaluations where detailed management data are comprehensively collected and systematically organized. The process-based model comparison reveals that while DNDC and LandscapeDNDC show similar performance under continuous flooding, they diverge significantly under Alternate Wetting and Drying (AWD) regimes. These discrepancies are primarily attributed to the models' different concepts of representing water table fluctuations.

Building on these results, the Tier 3 approach of LandscapeDNDC was integrated into the web‑based LUI‑RICE platform (https://ldndc.online/rice/). This makes GHG quantification for Vietnamese rice cultivation directly accessible to local stakeholders and policymakers, translating the scientific findings of this study into a practical decision-support application.

How to cite: Nguyen, C., Kraus, D., Nguyen, T., Wassmann, R., Butterbach-Bahl, K., Vo, T. B. T., Mai, V. T., Bui, T. P. L., and Kiese, R.: CH4 emissions in Vietnamese Rice Agriculture: Benchmarking process-based model approaches (Tier 3) against Tier 1/2 Estimates, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15692, https://doi.org/10.5194/egusphere-egu26-15692, 2026.

EGU26-15734 | Orals | AS3.38

ΔXCO/ΔXCO2 characteristics over coal-fire areas in Xinjiang, China using a portable EM27/SUN FTIR spectrometer 

Qiansi Tu, Jiaxin Fang, Frank Hase, André Butz, África Barreto, Omaira García, and Kai Qin

Long-term coal spontaneous combustion (CSC) represents a severe and persistent threat, resulting in substantial waste of energy resources, significant environmental degradation, and serious risks to human health and safety. To better understand the emission characteristics of CSC, we conducted ground-based measurements of XCO₂, XCH₄, XCO and aerosol optical depth (AOD) using a Fourier-transform infrared spectrometer (EM27/SUN) within the COCCON network, in the Wugonggou coal-fire region near Fukang, Xinjiang.

Our results indicate that TROPOMI satellite data systematically underestimated XCO, with a mean bias of 4.53 ± 5.53 ppb (4.54%). For distinct enhancement events observed by COCCON, ΔXCO₂ and ΔXCO exhibit a strong correlation (R² = 0.6082), with a slope of 9.782 ppb/ppm (9.782 × 10⁻³ ppm/ppm). This value is lower than the CAMS inventory ratio of 13.52 × 10⁻³. This discrepancy arises primarily from their distinct spatial representativeness. The COCCON instrument, located within the coal fire region, captures intense local combustion emission. In contrast, the CAMS product represents a daily average over a much larger model grid cell, which dilutes strong local point sources like coal fires within a broader regional background. Additionally, correlation analysis shows that ΔXCO is more closely linked to AOD (R² = 0.2283) than either ΔXCO₂ or ΔXCH₄, underscoring the distinct behavior of CO in coal-fire plumes.

How to cite: Tu, Q., Fang, J., Hase, F., Butz, A., Barreto, Á., García, O., and Qin, K.: ΔXCO/ΔXCO2 characteristics over coal-fire areas in Xinjiang, China using a portable EM27/SUN FTIR spectrometer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-15734, https://doi.org/10.5194/egusphere-egu26-15734, 2026.

EGU26-16089 | Orals | AS3.38

National-scale methane emissions in South Korea (2010–2021): insights from multiple inversion systems  

Samuel Takele Kenea, Daegeun Shin, Wonick Seo, Sunran Lee, Fenjuan Wang, Shamil Maksyutov, Rajesh Janardanan, Soojeong Lee, Dmitry A. Belikov, Prabir K. Patra, Nicole Montenegro, Antoine Berchet, Marielle Saunois, Adrien Martinez, Ruosi Liang, Yuzhong Zhang, Ge Ren, Hong Lin, Sara Hyvärinen, and Aki Tsuruta and the Sangwon Joo, Sumin Kim

Accurate estimation of methane (CH₄) emissions is essential for assessing mitigation progress, 
yet substantial uncertainties persist at the national scale. In South Korea, CH₄ emissions are 
predominantly anthropogenic, with the waste and agricultural sectors contributing 
approximately 82% of total national emissions. This study analyzes national-scale CH₄ 
emission estimates for South Korea during 2010–2021 using multiple atmospheric inversion 
systems participating in the Methane Inversion Inter-Comparison for Asia (MICA) project. 
Results from inversions using only in situ observations indicate that prior emissions over South 
Korea were likely overestimated. Prior estimates range from 1.5 to 1.7 Tg yr⁻¹ for most years, 
whereas posterior emissions are, on average, about 15% lower than the prior estimates. A 
notable exception is the LMDZ inversion model, which yields posterior estimates that are 40
67% lower than prior values. This substantial reduction is primarily associated with the waste 
sector. Sectoral attribution reveals substantial inter-model differences. LMDZ shows a 
decreasing waste-sector emission trend in Exp. 1 but an increasing trend when only satellite 
observations are assimilated (Exp. 2), whereas the STILT-based inversion consistently 
indicates increasing waste-sector emissions. Given that the waste sector dominates national 
CH₄ emissions, these discrepancies strongly influence total emission estimates. The prior 
waste-sector emissions, derived from EDGAR v7, exceed those reported in South Korea’s 
national greenhouse gas inventory (GIR), contributing to the observed overestimation. 
Additionally, the inversion-derived posterior estimates consistently indicate an overestimation 
of prior agricultural emissions during the summer months. Model performance evaluation over 
the region of interest indicates varying levels of agreement between simulated and observed 
CH₄ mole fractions, with correlation coefficients ranging from 0.24 to 0.85 and posterior biases 
ranging from −65.6 to 0.34 ppb, highlighting the choice of transport model is important. Overall, 
this study highlights the value of multi-model inversion inter-comparisons for constraining 
national-scale CH₄ emissions, diagnosing sector-specific uncertainties, and identifying 
structural differences among inversion frameworks that can guide future improvements. 

How to cite: Takele Kenea, S., Shin, D., Seo, W., Lee, S., Wang, F., Maksyutov, S., Janardanan, R., Lee, S., Belikov, D. A., Patra, P. K., Montenegro, N., Berchet, A., Saunois, M., Martinez, A., Liang, R., Zhang, Y., Ren, G., Lin, H., Hyvärinen, S., and Tsuruta, A. and the Sangwon Joo, Sumin Kim: National-scale methane emissions in South Korea (2010–2021): insights from multiple inversion systems , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16089, https://doi.org/10.5194/egusphere-egu26-16089, 2026.

EGU26-16769 | Posters on site | AS3.38

Improving the Accuracy of CO₂ Emission Estimates over South Korea Using a Top-down Inversion Framework 

Ho Yeon Shin, Daegeun Shin, Samuel Takele Kenea, Sunran Lee, Sumin Kim, and Yun Gon Lee

The international community has continuously monitored carbon emissions by publishing National Inventory Reports (NIRs) under the Paris Agreement adopted in 2015 to address the climate crisis. However, current emission estimation methods predominantly rely on bottom-up approaches based on statistical information, which are subject to limitations, including the potential omission of emission sources and the long time required for emission compilation. To overcome these limitations, top-down approaches that estimate emissions using meteorological models and observed atmospheric greenhouse gas concentrations have recently gained increasing attention. This approach has been adopted as a scientific methodology of the Integrated Global Greenhouse Gas Information System (IG3IS), developed under the auspices of the World Meteorological Organization (WMO), and is regarded as a complementary alternative to conventional emission inventories. In this study, carbon dioxide (CO₂) emissions over South Korea were estimated using a top-down approach based on the Stochastic Time-Inverted Lagrangian Transport Model (STILT) and observations from WMO/Global Atmosphere Watch (GAW) stations, and their accuracy was evaluated. The STILT-based inversion results indicate that anthropogenic CO₂ emissions in South Korea for 2019 amount to 589.7 Mt yr⁻¹, which is 83.6 Mt yr⁻¹ lower than the estimate reported in the existing NIR. The downward correction is primarily concentrated in Seoul and the surrounding metropolitan region. Furthermore, to account for the spatial characteristics of CO₂ emission distributions, high-resolution and realistic emission estimates were derived for regions with dense point-source emissions using the Weather Research and Forecasting (WRF) model. The application of top-down approaches for greenhouse gas emission estimation in East Asian countries, together with continuous technological advancement, is expected to provide a scientific foundation for improving the reliability of emission estimates and supporting future climate crisis response strategies.

How to cite: Shin, H. Y., Shin, D., Kenea, S. T., Lee, S., Kim, S., and Lee, Y. G.: Improving the Accuracy of CO₂ Emission Estimates over South Korea Using a Top-down Inversion Framework, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16769, https://doi.org/10.5194/egusphere-egu26-16769, 2026.

EGU26-17209 | Posters on site | AS3.38

Development and Application of a Cryogenic Preconcentration System for Halogenated Greenhouse Gas Measurements in Korea 

Joo-Ae Kim, Sunggu Kang, Dohyun Kwon, Sunyoung Park, Soojeong Lee, and Sumin Kim

East Asia represents a major source region of greenhouse gas emissions associated with rapid industrialization and increasing energy demand. Among these emissions, halogenated synthetic greenhouse gases such as HFCs and PFCs, which have been widely used as substitutes following international regulations for ozone layer protection, are characterized by high global warming potentials (GWPs).

In South Korea, halogenated greenhouse gases have been monitored at the Gosan station on Jeju Island using the MEDUSA system of the AGAGE network.  However, the expansion of observational coverage and the establishment of measurement capabilities remain essential to better characterize regional emission signals.  In this study, a cryogenic preconcentration and analysis capability for halogenated greenhouse gases (NIMS-preconcentrator) was developed and and evaluate its capability for monitoring halogenated greenhouse gases.

The analytical setup includes a cryogenic thermal desorption (TD) unit and a pre-concentration trap capable of reaching temperatures down to −170 °C, integrated with an automated valve control module and gas chromatography–mass spectrometry (GC–MS). Measurements were conducted using an offline canister-based sampling approach. Analysis of ambient air samples collected at Anmyeondo (GAW station) resolved about ten halogenated greenhouse gas species, including HFC-134a, HFC-125, and legacy chlorofluorocarbons such as CFC-11 and CFC-12. Concentrations were evaluated using calibration standards, and ongoing performance assessment is conducted using laboratory working standards employed at the Gosan AGAGE station.

This study aims to establish a new measurement capability for halogenated greenhouse gases and to assess its consistency with international observation. Continued operation of this system will support the accumulation of long-term observational datasets and facilitate regional-scale analysis and inter-comparison of high-GWP halogenated greenhouse gases in Northeast Asia.

How to cite: Kim, J.-A., Kang, S., Kwon, D., Park, S., Lee, S., and Kim, S.: Development and Application of a Cryogenic Preconcentration System for Halogenated Greenhouse Gas Measurements in Korea, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17209, https://doi.org/10.5194/egusphere-egu26-17209, 2026.

EGU26-17591 | Posters on site | AS3.38

High-resolution direct GHG emission estimation and simulation from residential space heating using open data  

Kirsten v. Elverfeldt, Gefei Kong, Veit Urlich, Maria Martin, Moritz Schott, and Sebastian Block

Residential space heating remains a major source of greenhouse gas emissions in the building sector. In Germany, space heating accounts for the largest share of residential energy consumption, and accurate quantification of associated emissions is essential to meet national climate mitigation targets.

Most research on residential heating emissions focuses on the regional or national levels, while estimates at finer spatial scales remain limited. Data availability further constrains the transferability and usability of current models. Consequently, approaches that deliver spatially and temporally detailed emission estimates and interactive tools to support analysis and decision-making by stakeholders are urgently needed.

We introduce the Climate Action Navigator (CAN), a dashboard for the analysis and visualization of climate mitigation and adaptation spatial data, based entirely on open science principles. One of the tools available in the CAN estimates carbon dioxide emissions from residential heating at fine spatial at temporal scales. The tool applies a bottom-up accounting methodology at 100 m spatial resolution based on publicly available census and building characteristics data in Germany, including building age and dominant energy carriers. The resulting emission estimates are consistent with official city- and national-level inventories, confirming methodological reliability. Germany-wide analyses reveal strong spatial heterogeneity in energy consumption and emissions that correlate with urban morphological characteristics.

Temporal dynamics are captured through an hourly simulation using the Demand Ninja model based on local weather data. The resulting temporal emission patterns can support inverse emission modelling applications as well as aid energy management by, for example, revealing peak heating demand times and locations.

Results are delivered via the CAN interface as intuitive, interactive maps and charts that allow users to compare across neighborhoods, explore temporal emission dynamics, and assess potential mitigation actions. By integrating open-source data with high-resolution modeling and visualization, the Climate Action Navigator bridges the gap between scientific emission quantification and practical decision making. The approach supports transparent attribution and tracking of residential space-heating emissions, thereby advancing evidence-based climate mitigation planning.

How to cite: v. Elverfeldt, K., Kong, G., Urlich, V., Martin, M., Schott, M., and Block, S.: High-resolution direct GHG emission estimation and simulation from residential space heating using open data , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17591, https://doi.org/10.5194/egusphere-egu26-17591, 2026.

EGU26-19274 | ECS | Posters on site | AS3.38

Carbon dioxide and methane emissions from a network of thirty eddy-covariance sites in the Netherlands 

Ignacio Andueza Kovacevic, Laurent Bataille, Isabel Cabezas, Freek Engel, Wietse Franssen, Corine van Huissteden, Ronald Hutjes, Ruchita Ingle, Wilma Jans, Tan JR Lippmann, Jeferson Zerrudo, Hong Zhao, Reinder Nouta, and Bart Kruijt

Understanding the temporal dynamics and controls on greenhouse gas exchange between terrestrial ecosystems and the atmosphere is critical for advancing process-level understanding and informing national greenhouse gas budgets and inventories. A large portion of soils in the Netherlands are either drained or restored peatlands, where the high carbon/organic matter content is accompanied by large risk of carbon loss to the atmosphere through enhanced soil respiration (drained sites) and/or enhanced methane emissions (rewetted sites). For this reason, increasing attention is being paid to understanding and quantifying the greenhouse gas budgets of both drained and restored peatland sites across the Netherlands. 
 
To both inform national GHG inventories and improve our understanding of site scale process, we present a multi-site analysis of a network of more than thirty eddy-covariance sites in the Netherlands. We discuss the daily, seasonal, and annual variability of carbon dioxide (CO₂) and methane (CH₄) fluxes measured at these sites. These sites include intensively managed grasslands, arable fields, semi-natural pastures, forested peatlands, wetlands and marshes. These sites encompass a wide range of vegetation types, soil characteristics, and water-management practices, with continuous or semi-continuous high-frequency flux datasets extending across multiple years within the last decade.
 
We quantify daily, seasonal, and annual CO₂ and CH₄ fluxes and discuss key biophysical drivers, including soil composition and moisture, vegetation dynamics, groundwater levels, and the impacts of climate anomalies such as temperature and precipitation extremes across varying timescales. We discuss differences between sites and potential impacts of soil characteristics, vegetation, land management, and recent climate anomalies.
 
Our analysis indicates substantial variability in both CO₂ and CH₄ fluxes across sites and seasons. These results highlight the invaluable contributions of both high-resolution flux observations and rigorous data processing methods when disentangling ecosystem controls on gas exchange. These flux observations provide much needed empirical constraints for model evaluation and can facilitate improved representation of peatland and wetland systems in greenhouse gas inventories and process-based models.

How to cite: Andueza Kovacevic, I., Bataille, L., Cabezas, I., Engel, F., Franssen, W., van Huissteden, C., Hutjes, R., Ingle, R., Jans, W., Lippmann, T. J., Zerrudo, J., Zhao, H., Nouta, R., and Kruijt, B.: Carbon dioxide and methane emissions from a network of thirty eddy-covariance sites in the Netherlands, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19274, https://doi.org/10.5194/egusphere-egu26-19274, 2026.

EGU26-19514 | Orals | AS3.38

Towards accurate quantification of New Zealand’s methane emissions from waste and agriculture 

Peter Sperlich, Christian Stiegler, Alex Geddes, Hamish Sutton, Brendon Smith, Molly Leitch, Sally Gray, Gordon Brailsford, Rowena Moss, Beata Bukosa, Sara Mikaloff-Fletcher, Amir Pirooz, Richard Turner, Jocelyn Turnbull, Johannes Laubach, Suzanne Rowe, Lorna McNaughton, Olivia Spaans, Kevan Brian, and Ellen Wymei

Methane emissions from waste and agriculture account for 46.6 % of Aotearoa New Zealand’s (ANZ) gross greenhouse gas emissions in 2023. Despite the significance of methane emissions, the only way to estimate their magnitude is based on emission factor methods, which include large uncertainties.  We present newly developed tools to directly measure methane emissions from wastewater treatment facilities, animal effluent storage systems and herds of dairy cows. We deploy in situ analysers on mobile observation platforms (vehicle and drone) and quantify methane emission fluxes using the tracer gas technique.  The accuracy of this method is estimated in multiple ways: i) a controlled release experiment, ii) through comparison to a mass-balance modelling approach, iii) through comparison to co-located chamber measurements for methane emissions from effluent ponds, iv) through comparison to co-located measurements of animal emissions using the “GreenFeed” technique. The comparisons show excellent agreement, providing much needed assurance of analytical performance to our mobile techniques. Our tools support ANZ’s farmers and waste managers to better understand current emissions, as well as to assess the efficacy of investments into emission mitigation. Additional tests explore new isotope techniques with the goal to quantify methane fluxes from different components within a plant, for example methane derived from digestors versus methane derived from biosolids in wastewater treatment systems, or methane from the open face of a landfill versus emissions from an area that is covered.

How to cite: Sperlich, P., Stiegler, C., Geddes, A., Sutton, H., Smith, B., Leitch, M., Gray, S., Brailsford, G., Moss, R., Bukosa, B., Mikaloff-Fletcher, S., Pirooz, A., Turner, R., Turnbull, J., Laubach, J., Rowe, S., McNaughton, L., Spaans, O., Brian, K., and Wymei, E.: Towards accurate quantification of New Zealand’s methane emissions from waste and agriculture, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19514, https://doi.org/10.5194/egusphere-egu26-19514, 2026.

EGU26-19832 | ECS | Orals | AS3.38

Can observation-based atmospheric mixing state reduce filtering sensitivity in GHG inversions? Lessons from the UK GEMMA programme 

Dafina Kikaj, Peter Andrews, Alexandre Danjou, Alistair Manning, Matt Rigby, Ed Chung, Grant Forster, Angelina Wenger, Chris Rennick, Emmal Safi, Simon O’Doherty, Kieran Stanley, Joe Pitt, and Tom Gardiner

Uncertainty in atmospheric transport models, especially boundary-layer mixing and turbulence, still limits confidence in top-down GHG emission estimates. In inversion workflows, observation selection is commonly supported by empirically tuned filters based on modelled meteorological variables (e.g., boundary-layer height, wind speed). The selection prioritises periods when transport is expected to be well represented. This motivates continued work to characterise atmospheric mixing and its associated uncertainties using observations.

In the UK GEMMA programme, we investigate whether observation-based atmospheric mixing state can provide complementary information to support uncertainty characterisation in UK CH₄ inversions. We demonstrate the framework at UK sites with radon measurements and at a newly instrumented site in Scotland where only meteorological measurements are available. Where radon is measured, we use it as an independent tracer of near-surface mixing and compare observed radon with radon simulated using the Met Office NAME dispersion model and a radon flux map. This comparison is used to define transport-performance classes (periods of relatively better vs poorer agreement) and associated atmospheric mixing state. At the Scotland site, we derive atmospheric mixing regimes from in situ meteorological measurements alone, using a vertical profile sampled every 10 m to characterise stratification and mixing.

We show how the resulting atmospheric mixing state and transport-performance classes can be used in two operational ways: (i) as additional information to support observation selection alongside existing practice, and (ii) to define regime-dependent uncertainty characterisation within inversion frameworks rather than assuming a single fixed error model. We illustrate the approach using two UK CH₄ inverse methods (InTEM and RHIME) and discuss how observation-based mixing information can improve transparency and reproducibility in hybrid (inventory + atmospheric) emissions estimation for IG3IS-aligned information services.

How to cite: Kikaj, D., Andrews, P., Danjou, A., Manning, A., Rigby, M., Chung, E., Forster, G., Wenger, A., Rennick, C., Safi, E., O’Doherty, S., Stanley, K., Pitt, J., and Gardiner, T.: Can observation-based atmospheric mixing state reduce filtering sensitivity in GHG inversions? Lessons from the UK GEMMA programme, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19832, https://doi.org/10.5194/egusphere-egu26-19832, 2026.

EGU26-20089 | Posters on site | AS3.38

From GHG Observations to Actionable Climate Information Services 

Daphne Kitsou, Parakevi Chantzi, Dimitrios Gkoutzikostas, Vasileios Rousonikolos, Georgios Galanis, Argiro Papastergiou, and Georgios Zalidis

Effective climate mitigation requires obtaining greenhouse gas (GHG) information and accounting that is scientifically robust and actionable for decision-making. The CARBONICA project has developed and implemented a robust climate-positive action plan for carbon farming implementation across the widening countries of Greece, Cyprus and North Macedonia, generating climate information services that operate at regional, national, and international scales. An extended management practices inventory has been developed and implemented in pilot sites across 15 crops between the 3 countries, fully aligned with the IPCC, the Natural Climate Solutions World Atlas, the GHG Protocol, and climate related EU laws and initiatives. GHG accounting is supported by a robust MRV system combining soil sampling, field inputs following IPCC Scope guidance, and management practices, covering direct, indirect, and upstream emissions across the farm system, with all procedures are fully compliant with ISO 14064-2. Farm-level data are also collected using the validated Field Diagnostic Toolbox, which includes soil CO₂ flux monitoring using spectroscopy to support accurate assessment of emissions and carbon removals.

This enables explicit attribution of emissions and carbon removals to farms, regions, and in general, the agrifood sector, supporting monitoring, reporting and validating of mitigation measures for positive climate action. LCA modelling on a pilot site (1ha peach orchard) has shown significant results in emissions reductions and carbon removals. The model was used once on the baseline (business-as-usual scenario) in 2024, and once after the management practices no- till and residues incorporation were implemented in the orchard, for the year 2025. The total greenhouse gas emissions from the pilot peach orchard decreased from 2,660 kg CO₂e in 2024 to 1,280 kg CO₂e in 2025, with emissions per ton of produced fruit dropping from 147.63 kg CO₂e to 71.04 kg CO₂e. Beyond the reduction of the emission sources, the demonstrated change in the soil carbon stock was also significant. While the 2024 cultivation season showed a net-zero change compared to the baseline scenario, the implementation of no-till and crop residue incorporation during the 2025 season created an active carbon sink, resulting in a net removal of 597.76 kg of CO₂e from the atmosphere into the soil. Thus, the project successfully demonstrated a twofold climate benefit: a major reduction in operation emissions and a significant sequestration of atmospheric carbon into the soil.

The results presented above are part of a third-party validated carbon farming project, facilitated through CARBONICA. This work also contributes to IG3IS-aligned applications demonstrating the operational use of multi-source GHG observations for real-world solutions in carbon farming.

How to cite: Kitsou, D., Chantzi, P., Gkoutzikostas, D., Rousonikolos, V., Galanis, G., Papastergiou, A., and Zalidis, G.: From GHG Observations to Actionable Climate Information Services, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20089, https://doi.org/10.5194/egusphere-egu26-20089, 2026.

EGU26-20826 | ECS | Orals | AS3.38

Daily and 1/16 degree maps of CO2 fossil fuel emissions based on satellite retrievals of pollutant atmospheric data 

Alexandre Héraud, Frédéric Chevallier, Grégoire Broquet, Philippe Ciais, Adrien Martinez, and Anthony Rey-Pommier

In the context of the Paris Agreement on climate change and of a global effort to reduce greenhouse gas emissions, the monitoring of anthropogenic carbon dioxide (CO2) emissions is needed to assist policy makers but represents a major challenge. While current inventories provide rather robust annual emission totals at country scale, they lag behind real time by many months and they lack spatial and sub-annual details. Here we map the daily surface fossil fuel CO2 emissions at a 1/16 degree resolution over Europe, with the year 2021 as an example, based on spaceborne atmospheric composition observations.

As the high-resolution satellite monitoring of atmospheric CO2 remains challenging, especially at a local spatial scale and a daily time scale, we take advantage of the co-emission of CO2 and nitrogen oxides (NOX) during fossil fuel combustion: we exploit images of nitrogen dioxide (NO2) concentrations retrieved from the measurements of the Tropospheric Monitoring Instrument (TROPOMI) onboard the Sentinel-5P satellite.

From the TROPOMI NO2 concentrations, we retrieve daily maps of NOX emissions based on the divergence of the mass fluxes within the NO2 images. We combine the changes of these maps from one year to the next with low latency national CO2 emissions from Carbon Monitor (https://carbonmonitor.org/), and with a baseline of monthly spatially-distributed CO2 emissions for a previous year (here 2020) from GridFED (https://mattwjones.co.uk/co2-emissions-gridded/) from which we removed aviation and shipping emissions beforehand.

The resulting maps of emission increments from 2020 to 2021 capture changes in highly emitting areas: major urban or industrial areas, and main transport corridors. The emissions for the year 2021 show good consistency with existing inventories. The dataset also produces realistic seasonal variability at a local scale and captures daily variability, although temporally smoothed due to a 5-day rolling average of Carbon Monitor data.

This method is both temporally and spatially scalable and can therefore be extended to the entire world and to additional years, which provides encouraging prospects for the continuation of this work.

How to cite: Héraud, A., Chevallier, F., Broquet, G., Ciais, P., Martinez, A., and Rey-Pommier, A.: Daily and 1/16 degree maps of CO2 fossil fuel emissions based on satellite retrievals of pollutant atmospheric data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20826, https://doi.org/10.5194/egusphere-egu26-20826, 2026.

Quantitative evidence is increasingly required to assess the mitigation potential of cities in achieving global carbon neutrality. However, although urban green spaces contribute simultaneously through biophysical carbon sequestration and reductions in energy demand driven by urban heat island mitigation, few studies have systematically compared and evaluated these two effects within a unified framework at the global scale.This study quantifies the total contribution of urban green spaces to carbon neutrality across global cities and decomposes this contribution into carbon sequestration and cooling driven energy savings, assessing their relative importance and spatial patterns.The urban heat island effect is estimated using remote sensing derived land surface temperature differences between urban and non urban areas, while carbon sequestration by urban green spaces is simultaneously quantified based on satellite based observations.These two contributions are then integrated and compared. Furthermore, this study examines how the relative importance of the two effects varies across major climate zones and how heterogeneity manifests in distinct spatial patterns. Finally, this study investigates how vegetation related indicators, socio economic variables, and urban structural characteristics influence the two effects across climate zones with AI based approaches and identify contextual conditions under which the mitigation benefits of urban green spaces are amplified or attenuated even under similar urban green space availability.This study provides a global assessment of the contribution of urban green spaces to carbon neutrality and offers empirical evidence to support the design of climate and context specific nature based mitigation strategies in cities.

How to cite: Kim, S. and Choi, Y.: The dual role of urban green spaces in carbon neutrality: carbon sequestration and cooling driven energy savings at the global scale, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20959, https://doi.org/10.5194/egusphere-egu26-20959, 2026.

EGU26-22515 | Orals | AS3.38 | Highlight

Assessing the accuracy of the Climate Trace global vehicular and power plant CO2 emissions 

Kevin Gurney, Bilal Aslam, Pawlok Dass, Lech Gawuc, Toby Hocking, Jarrett Barber, and Anna Kato

Accurate estimation of greenhouse gas (GHG) emissions at the infrastructure scale remains essential to climate science and policy applications. Powerplant and vehicle emissions often form the majority of fossil fuel CO2 (FFCO2) emissions in much of the world at multiple scales. Climate Trace, co-founded by former U.S. Vice President Al Gore, is a new AI-based effort to estimate pointwise and roadway-scale GHG emissions, among other sectors. However, limited independent peer-reviewed assessment has been made of this dataset. Here, we update a previous analysis of Climate Trace powerplant FFCO2 emissions in the U.S. and present a new analysis of Climate Trace urban on-road CO2 emissions in U.S. urban areas. This is done through comparison to an atmospherically calibrated, multi-constraint estimates of powerplant and on-road CO2 emissions from the Vulcan Project (version 4.0).

Across 260 urban areas in 2021, we find a mean relative difference (MRD) of 69.9% in urban inroad FFCO2 emissions. Furthermore, differing versions of the Climate Trace on-road emissions releases shift from over to under-estimation in almost equal magnitudes. These large differences are driven by biases in Climate Trace’s machine learning model, fuel economy values, and fleet distribution values. An update to the powerplant FFCO2 emissions analysis (from a 2024 paper) show both improved and degraded convergence of emissions. We continue to recommend that sub-national policy guidance or climate science applications using the GHG emissions estimates in these sectors made by Climate Trace should be done so with caution.

How to cite: Gurney, K., Aslam, B., Dass, P., Gawuc, L., Hocking, T., Barber, J., and Kato, A.: Assessing the accuracy of the Climate Trace global vehicular and power plant CO2 emissions, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-22515, https://doi.org/10.5194/egusphere-egu26-22515, 2026.

EGU26-273 | ECS | Posters on site | ERE4.1

Sulfur, Carbon, and Oxygen Isotope Constraints on Fluid Sources at the Tamdroust Cu Ore Deposit (Central Anti-Atlas) 

Ismail Bouskri, Said Ilmen, Mustapha Souhassou, Moha Ikenne, Abdel-Ali Kharis, Mohamed Hibti, Abdelaziz Gaouzi, Mohamed Zouhair, Lhou Maacha, Sajjad Maghfouri, Marieme Jabbour, Mohammed Ouchchen, and Mbarek Ghannami

The Tamdroust copper ore deposit, located within the Bou Azzer–El Graara inlier (Central Anti-Atlas, Morocco), exemplifies Lower Cambrian carbonate–siliciclastic–hosted copper mineralization formed through the combined effects of stratigraphic, structural, and hydrothermal processes. The deposit lies within the Lower Cambrian Igoudine and Amouslek formations of the Tata Group. It is controlled by a major fault system trending N110°–N150°, which served as the main pathway for metalliferous fluids during Hercynian tectonic reactivation. Copper mineralization predominantly occurs in reduced green siltstones and dolostones deposited on a shallow, mixed carbonate–siliciclastic marine platform influenced by episodic terrigenous input. Two main styles of mineralization are recognized: (i) disseminated sulfides, including fine-grained bornite, chalcopyrite, and pyrite dispersed within permeable host rocks; and (ii) vein and veinlet stockworks along interconnected fracture corridors associated with the major fault zone. Textural and petrographic studies reveal a multi-stage paragenetic sequence evolution that comprises: (1) early disseminated and veinlet-type bornite–chalcopyrite–pyrite associated with quartz–calcite; (2) hydrothermal enrichment along faults marked by bornite replacement by chalcocite with digenite and covellite; and (3) supergene weathering producing native copper and secondary carbonates. Stable isotope geochemistry offers crucial insights into the origin and development of mineralizing fluids. Sulfur isotope compositions of bornite (δ³⁴S ≈ +10.2‰) suggest a mixed sulfur reservoir primarily formed by thermochemical sulfate reduction (TSR) of evaporitic sulfates, aligning with the presence of Lower Cambrian evaporite-rich formations. Carbon and oxygen isotope values measured in hydrothermal calcite (δ¹³C = –3.6 to –2.6‰ VPDB; δ¹⁸O = –15.8 to –15.2‰ VPDB, equivalent to +14.7 to +15.3‰ VSMOW) indicate moderate-temperature (~150–160°C) hydrothermal fluids originating from mixed meteoric–basinal brines that have isotopically equilibrated with carbonate–evaporite host rocks. The δ¹³C signatures further point to a dominant marine carbonate source with no significant biogenic carbon contribution, while minor meteoric or atmospheric mixing remains possible. These findings support a model of fluid–rock interaction in a mesothermal hydrothermal setting, where brines, partially modified by evaporites, played a key role in copper transport and sulfide formation. The spatial distribution of ores highlights the significance of redox-controlled mineralization, with the most notable mineral deposits forming at the boundary between oxidized hematite-bearing red beds and reduced green siltstones and carbonates. This redox boundary served as a chemical trap, allowing TSR-driven production of reduced sulfur species and subsequent copper sulfide deposition. In summary, geological, structural, and isotopic evidence indicate that the Tamdroust deposit is a carbonate-hosted copper system of epigenetic stratabound type in Cambrian evaporitic settings, formed during the Hercynian reactivation of Cambrian sedimentary basins. The Tamdroust system exhibits strong similarities with other Cambrian Cu ore deposits in the Anti-Atlas, particularly Jbel N’Zourk and Jbel Laassal, supporting a regional metallogenic model involving fault-controlled brine flow, evaporite involvement, and redox-driven sulfide formation. These findings offer a predictive framework for future copper exploration, focusing on structurally controlled brine pathways and redox boundaries as primary targets across the Central Anti-Atlas.

How to cite: Bouskri, I., Ilmen, S., Souhassou, M., Ikenne, M., Kharis, A.-A., Hibti, M., Gaouzi, A., Zouhair, M., Maacha, L., Maghfouri, S., Jabbour, M., Ouchchen, M., and Ghannami, M.: Sulfur, Carbon, and Oxygen Isotope Constraints on Fluid Sources at the Tamdroust Cu Ore Deposit (Central Anti-Atlas), EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-273, https://doi.org/10.5194/egusphere-egu26-273, 2026.

Deep longwall mining in North China-type coalfields is increasingly threatened by water inrush from high-pressure karstic limestone aquifers beneath the coal seam floor. Conventional grouting from underground roadways often has low pressure, short diffusion distances and poor control of hidden faults and collapse columns, so residual water-conducting channels may still trigger serious inflows. This contribution presents an integrated control mode and a quantitative verification framework for deep coal seam floor water hazards. First, a GIS-based multi-criteria assessment of floor failure depth, aquifer pressure and structural complexity is used to delineate high-risk blocks at panel scale. These blocks are treated in advance through coordinated control of water-filled aquifers and water-conducting structures, combining high-capacity directional drilling from the surface with supplementary underground boreholes to grout target limestone aquifers and associated fracture zones ahead of mining. To evaluate the effectiveness of the treatment before face retreat, we establish a sequential verification method that links borehole pressure tests, calculated water-blocking coefficients, repeated mine DC-resistivity surveys, spatial analysis of grouting pressure and volumes, and inspection drilling and inflow monitoring. Application to a >800 m deep longwall panel mining the 11# coal seam shows that inflows from overlying and underlying limestone aquifers were reduced to tens of cubic metres per hour and no floor water inrush occurred during mining. The proposed control–verification scheme provides a transferable engineering model for designing and auditing floor water-hazard management in deep coal mines affected by high-pressure confined aquifers.

How to cite: Hu, Y.: Integrated control and sequential verification of deep coal seam floor water inrush hazards, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-352, https://doi.org/10.5194/egusphere-egu26-352, 2026.

The Ni-Cu-Co mineralization in the Ringerike Municipality, Norway, is associated with a suite of magmatic intrusions occurring within the Eastern Kongsberg Complex (EKC). The complex formed during the Gothian Orogeny (1.6 - 1.5 Ga), and the most significant local Ni-Cu deposits are predominantly correlated with this magmatism (Orvik et al. 2025). Historically, nickel and copper were produced in this area until operations ceased in 1920 (Mathiesen & NGU, 1977).

In recent years, both industry and academia have shown renewed interest in the region. Current publications have advanced the understanding of the tectonic evolution of the EKC, and its implications for mineral exploration (Orvik et al. 2025). Mansur et al. (2025) discussed the formation and constraints of the most significant past producers, the Ertelien and Langedalen deposits. However, other than several master theses, there has been little to no focus on the other magmatic intrusions hosting the mineralization; the mineralization itself; and the local structural framework and controls on fluid flow. The current license holder, Kuniko Limited, carried out a range of exploration activities and defined a mineral resource estimate (MRE) for the Ni-Cu-Co Ertelien deposit (Kuniko Limited, 2024). The remaining magmatic intrusions received less attention, with large but disparate datasets being produced over the years.

This PhD aims at utilizing the collected data, supported by field and laboratory work, to understand the structural regime across the region and increase the understanding of the controls on mineralization. The integration of the available data will be undergone by application of python-based machine learning to generate mineral prospectivity mapping model. This would allow the identification of exploration targets and the development of hypotheses, which could be then tested by state-of-the-art exploration techniques, significantly enhancing the exploration efforts within the region.

References

Orvik, A. A., Mansur, E. T., Henderson, I., Slagstad, T., Huyskens, M. & Bjerkgård, T., 2025. Isotopic identification of paleo rift zones within the Sveconorwegian Province; implications for nickel sulphide utilisations in the SW Fennoscandian Shield. Precambrian Research 427, 107836.

Mansur, E., Orvik, A. A., Henderson, I., Miranda, A. C., Slagstad, T., Dare, S., Bjerkgard, T., Sandstad, J. S., 2025. Formation of the Ertelien and Langedalen magmatic Ni–Cu sulfide deposits in Norway: investigating the evolution of platinum-group-element-depleted systems at convergent margins. European Journal of Mineralogy 37, 841869

Mathiesen, C. O. & The Geological Survey of Norway, 1977. Vurdering Av Ringerike Nikkelfelter. NGU-RAPPORT, 21.

Kuniko Limited, 2024. ASX Release: Significant Mineral Resource Increase at Ertelien. https://kuniko.eu/asx-announcements/

How to cite: Mroz, R.: Understanding the regional structural framework and controls on Ni-Cu-Co mineralization, in the Ringerike Metallogenic Province, Norway; , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-1191, https://doi.org/10.5194/egusphere-egu26-1191, 2026.

Introduction: This work deals with the regionalized classification of hydrothermal alteration types from data of continuous features (assays of trace elements and sulfide minerals) in a porphyry copper-gold deposit in Mongolia, using supervised learning algorithms. Traditional machine learning methods ignore the spatial correlations of regionalized data, whereas geostatistics can take advantage of these correlations and enhance classification scores. The novelty of our proposal lies in the deployment of a complementary set of features (‘proxies’) at the sampled data points, calculated ingeniously through geostatistical simulation with nugget effect filtering. 

Methodology: We perform the cleaning and preparation of a vast set of exploratory drill hole samples, including the splitting of this dataset into training and testing subsets in the ratio 70:30. The dataset is used for the geostatistical modeling of the feature variables to simulate (by spectral simulation with filtering) the same feature variables at the training and testing data points. Because of the nugget effect filtering, the simulated values ('proxies') do not coincide with the measured (noisy) values and exhibit a stronger spatial continuity. The proxies are then taken as the input for a supervised classification of the hydrothermal alteration type on the training data, which incorporates misclassification cost matrices that account for geological criteria. The performance of the classifier is finally assessed on the testing data on the basis of standard metrics.

Results and Conclusions: Compared to the traditional approach, where hydrothermal alteration types are predicted directly from the measured features, the classification that uses the geostatistical proxies systematically provides better scores (accuracy rate and Cohen’s kappa statistic increased by 5 to 10 percentual points), showing the importance of incorporating proxy variables obtained by a spatial processing of the input information. Another advantage of using geostatistical proxies in the classification is the handling of missing data, insofar as these proxies provide a ‘clever’ alternative to the imputation of missing values, based on the spatial correlation structure of the feature variables and neighboring information, instead of a simple median value by alteration class. The use of geostatistical proxies can therefore be decisive in the presence of highly heterotopic datasets, for which discarding missing data implies a considerable loss of information. In a nutshell, our study demonstrates two things: the first is how geostatistics enriches machine learning to achieve higher predictive performance and to handle incomplete and noisy datasets in a spatial setting. Secondly, it establishes that better prediction accuracy can be achieved than in previous studies, where alteration types were predicted solely from geochemical data.

The proposed approach has far-reaching consequences for decision-making in mining exploration, geological modeling, and geometallurgical planning. We expect it to be used in supervised classification problems that arise in varied disciplines of natural sciences and engineering and involve regionalized data.

 

How to cite: Borah, A. and Emery, X.: Integration of Machine Learning and Geostatistics for Hydrothermal Alteration Classification in Smart Mining, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-2073, https://doi.org/10.5194/egusphere-egu26-2073, 2026.

Accurate and efficient rock mass characterization is crucial for achieving sustainable mineral exploration and resource evaluation, especially in the context of increasing global resource scarcity and the urgent need to reduce environmental and operational costs. The Rock Quality Designation (RQD) is a widely used indicator for assessing rock mass integrity in geological and geotechnical engineering. However, conventional RQD determination relies heavily on manual measurements of drill cores, which suffer from low efficiency, poor scalability, and limited integration into data-driven exploration workflows.

To address these limitations, this study proposes an automated approach for RQD computation of drill cores based on computer vision and deep learning. The method integrates image-based sensing with advanced object detection and image segmentation algorithms to achieve non-destructive and automated characterization of drill cores.

First, perspective correction is applied to field-acquired core images to ensure geometric consistency. The principle of perspective correction is to project the two-dimensional original image into a three-dimensional viewing space and then transform the three-dimensional space to the image processing plane. The formulas are as follows:

The 3D viewing space is then mapped to the image processing plane using:

Subsequently, the Segment Anything Model (SAM) is employed to automatically detect and extract core regions based on the similarity of color and texture features. In SAM, the prompt encoder partitions and encodes the image based on object color, texture, and other features using:

On this basis, a YOLOv8-based image segmentation model is constructed to identify gap features between core pieces, enabling precise segmentation of individual core segments. YOLOv8 selects positive samples using the TaskAlignedAssigner strategy, formulated as:

Furthermore, by establishing a mapping between image pixels and physical dimensions, the lengths of core pieces are automatically quantified, enabling RQD computation as follows:

Studies on practical cases indicate that this approach maintains high computational accuracy while significantly improving processing efficiency, highlighting its potential as an AI-driven tool for automated core characterization. This method provides a scalable, non-destructive, and efficient technique for digital and data-driven mineral exploration workflows, supporting more sustainable and scientifically informed decision-making in mineral exploration and resource evaluation.

How to cite: Jiang, J.: Non-destructive, AI-based Rock Core Characterization for Automated RQD Assessment in Mineral Exploration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3464, https://doi.org/10.5194/egusphere-egu26-3464, 2026.

Electrical Resistivity Tomography (ERT) provides an effective means for probing the internal electrical structure of rock cores and plays an important role in understanding the electrical properties of ore-related geological bodies. Recovering informative structural representations from limited and highly coupled measurement data, however, remains challenging, particularly for drill cores, where complex resistivity distributions are commonly observed. Restricted electrode configurations and scale effects further hinder the ability of conventional inversion schemes and existing convolutional neural network (CNN)–based approaches to preserve structural continuity and spatial correlations in core-scale ERT imaging.

In this study, we investigate a dual-branch CNN–Transformer architecture designed for learning electrical structure representations from core-scale ERT data. The proposed approach adopts an end-to-end image-to-image learning paradigm to explore how complementary data organizations can be leveraged for representation learning. Two dedicated Transformer branches are incorporated: the first branch exploits potential difference data acquired from multiple sets of sequentially excited adjacent electrode pairs with consistent relative spatial configurations, while the second branch utilizes potential difference measurements collected at multiple spatial locations under a single electrode excitation.

By integrating the local feature extraction capability of CNNs with the global dependency modeling strength of Transformers, the proposed architecture aims to construct more expressive representations of complex electrical structures, thereby supporting improved structural coherence and spatial resolution in ERT imaging. Preliminary results, evaluated using quantitative imaging metrics including correlation coefficient and structural similarity index, suggest that the learned representations capture coherent electrical features under varying anomaly geometries, resistivity contrasts, and spatial distributions. These early findings demonstrate the feasibility of combining CNNs and Transformers for electrical structure representation learning in core-scale ERT and provide a methodological foundation for subsequent development of effective deep learning–based inversion strategies oriented toward deep mineral exploration applications.

This work is supported by National Science and Technology Major Project for Deep Earth Probe and Mineral Resources Exploration under Grant 2025ZD1008500.

How to cite: Shen, W., Zou, C., and Peng, C.: Learning Electrical Structure Representations from Ore-Bearing Cores ERT Data Using a Dual Branch CNN Transformer Architecture, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7353, https://doi.org/10.5194/egusphere-egu26-7353, 2026.

Surface wave signals between station pairs can be obtained by cross-correlating long-term continuous ambient noise recordings, from which group- and phase-velocity dispersion measurements at different periods are obtained and subsequently inverted for 3-D shear-wave velocity structures from shallow crust to upper mantle. This method does not rely on artificial seismic sources such as explosives, features relatively low exploration costs, and is well suited to complex topographic and environmental conditions. In recent years, it has been widely applied to image 3-D isotropic shear-wave velocity structures of mineral districts at different spatial scales (Hollis et al., 2018; Zheng et al., 2022; Jing et al., 2025). However, due to limitations in imaging resolution and the relatively small density contrast between ore-related rock bodies and surrounding host rocks, isotropic velocity structures alone are often insufficient for the effective identification and detailed characterization of ore-related rock bodies.

To address these limitations, we employed a direct surface wave tomography framework (Fang et al.,2015; Liu et al., 2019) to a selected mineral district using dense array ambient noise data. We first resolved the 3-D isotropic shear-wave velocity structure and subsequently retrieved the azimuthally anisotropic velocity structure in the very shallow crust. The results demonstrate that the isotropic velocity structure clearly delineates the major ore-controlling faults and structural framework of the mineral district, providing insights into its ore-forming tectonic regime. Besides, the azimuthally anisotropic shear-wave velocity structure shows strong spatial consistency with the distribution of known ore-related rock bodies and effectively highlights potential favorable mineralization targets. Overall, our study suggests that the combined interpretation of 3-D isotropic and azimuthally anisotropic velocity structures derived from ambient noise surface wave tomography provides an effective geophysical tool for mineral exploration and evaluation at both shallow and deep levels in mineral districts.

Reference

[1] Hollis D, McBride J, Good D, et al. 2018. Use of ambient-noise surface-wave tomography in mineral resource exploration and evaluation. SEG Technical Program Expanded Abstracts: 1937-1940.

[2] Zheng F, Xu T, Ai Y S, et al. 2022. Metallogenic potential of the Wulong goldfield, Liaodong Peninsula, China revealed by high-resolution ambient noise tomography. Ore Geology Reviews, 142: 104704.

[3] Jing J L, Chen G X, Li P, et al. 2025. Ambient noise seismic tomography of Tonglushan skarn-type Cu-Fe-Au deposit in Eastern China. Ore Geology Reviews, 184: 106718.

[4] Fang H J, Yao H J, Zhang H J, et al. 2015. Direct inversion of surface wave dispersion for three-dimensional shallow crustal structure based on ray tracing: methodology and application. Geophysical Journal International, 201(3): 1251-1263.

[5] Liu C M, Yao H J, Yang H Y, et al. 2019. Direct inversion for three-dimensional shear wave speed azimuthal anisotropy based on surface wave ray tracing: Methodology and application to Yunnan, southwest China. Journal of Geophysical Research: Solid Earth, 124(11): 11394-11413.

How to cite: Fang, J., Li, X., Yao, H., and Luo, X.: Azimuthal Anisotropy of Ambient Noise Rayleigh Waves Revealing Ore-Controlling Structures and Ore-Related Rock Bodies in a Mineral District, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7639, https://doi.org/10.5194/egusphere-egu26-7639, 2026.

With a focus on geo-modeling applications for sustainable deep mineral exploration, we propose affordable, but still accurate subsurface modeling technique that can generates realistic 3-D geological models. Conventional geostatistical methods based on two-point statistics, often compromise their performance in deep and structurally complex geological settings mostly due to limitation in modelling complex spatial continuity patterns. On the other hand, deep generative modelling techniques, such as generative adversarial networks (GAN), allow to predict complex spatial patterns but have difficulties to create large-scales models in three-dimensions and be locally conditioned by observations.

We introduce a deep generative framework that adapts conditional GANs with spatially adaptive normalization (cGAN–SPADE) for 3-D geological modeling under sparse and evolving data conditions to predict high resolution subsurface models with real-time data assimilation capabilities. The goal is to generate geo-models based on a priori geological information (i.e., expected geometries and probability maps) with real-time model update as new data are acquired during drilling.

The cGAN-SAPDE is trained with samples based on prior geological knowledge and existing borehole experimental data. Training proceeds through a generator and discriminator scheme in which generator produces new models based on input training data while the discriminator output is the probability of input image being real based on the corresponding conditioning map.

A conditioning map is introduced at each generator’s layer, where it modulates the intermediate activations using SPADE normalization. This mechanism injects spatially varying conditioning information into the network, enabling the generator to preserve structural coherence and fine-grained spatial details in the synthesized outputs.

Experimental results on industry-standard challenging 3-D synthetic data sets show the ability of the network to predict high-resolution 3-D geological models that simultaneously match a priori information and direct measurements acquired in real-time scenario.

This project has received funding from the European Union’s Horizon Europe Research and Innovation Program under the Grant Agreement No.101178775

How to cite: Akram, N. and Azevedo, L.: AI-driven framework to reconstruct real-time 3-D geological models for In-Situ Exploration of Critical Raw Materials, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7960, https://doi.org/10.5194/egusphere-egu26-7960, 2026.

The study area is located in the Eastern Taurus Belt, north of the Keban Reservoir Lake, between the districts of Pertek and Çemişgezek in the province of Tunceli. In the Eastern Taurus Belt, mineralizations are widespread associated with the intrusion of magmatic intrusions into carbonate-rich rocks. The studied zone reflects mineral associations that developed primarily due to iron-bearing minerals associated with skarn formations. The skarn formations developed between the Keban Metamorphics (Permo-Triassic) and the Pertek Granitoid (late Cretaceous) are approximately E-W trending and observed in a narrow line in the region. The most common iron-bearing mineral groups in the area are mainly found as magnetite or ilmenite, as alteration minerals are limonite, hematite ± actinolite. Remote sensing methods were tested to support classical methods in tracking the distribution and traces of these mineralizations. In this context, work was carried out to detect iron-rich zones (FeOx) along the Pertek-Çemişgezek (Tunceli) line. The composite images were used for this region, referencing known iron zones, by the ASTER satellite and image enhancement methods. Accordingly, the main target areas in the southern part of Tunceli province were determined as Köçek Village, Çemişgezek Ferry Terminal in the southwest, the area between Kolankaya and Çataksu in the southeast, and the area bounded by Tozkoparan in the northeast. The image from the ASTER satellite (AST_L1T) was cropped according to the study area, and all work was performed on this dataset. The cropped image set has been limited to fit the workspace. All work was performed using the VNIR and SWIR bands of the ASTER images. Radiometric corrections were made on the relevant dataset, and spectral anomalies were minimized. The VNIR spectral bands, which have a 15-meter ground resolution, were downsampled to a 30-meter ground resolution and balanced with the SWIR spectral bands. By comparing with known ground control points, RGB composite images showing the iron-rich zones in the region were created using different band combinations. As a result, it was determined that VNIR Band 2 / VNIR Band 1, SWIR Band 6, and VNIR Band 3 had the best combinations. In the controls performed, a 94% correlation was tested over the observation points and known iron occurrences. Ultimately, known mineralized zones were found to contain both iron-bearing and iron-rich zones. They were observed primarily Ayazpinari iron (Fe) occurrences, Ballıdut FeOx Alterations, and Çemişgezek Elazığ Road Cut FeOx alterations by both satellite observations and field verification studies. 

Note: This study was supported by Fırat University project MF-25.09.

How to cite: Tutlu, R., Ural, M., and Eğri, M.: Detection of Iron-Rich Zones Developed By Skarnification In The Cemisgezek-Pertek (Tunceli) Region Using Remote Sensing Methods, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8118, https://doi.org/10.5194/egusphere-egu26-8118, 2026.

EGU26-8405 | Posters on site | ERE4.1

Point cloud segmentation of sedimentary facies in outcrops with convolutional neural networks 

Ítalo Gonçalves, Ezequiel de Souza, Felipe Guadagnin, Eduardo Roemers-Oliveira, Ester Machado, Guilherme Rangel, Ana Clara Freccia, Jean Toledo, Gabriel Schaffer, and Claiton Scherer

3D point clouds of outcrops are digital representations of rock exposures used for geological surveying. These datasets often have high spatial density, up to a thousand points per square meter. By integrating georeferenced data into the 3D point cloud and applying remote sensing interpretation techniques, geoscientists can extract geological features and build 3D models. These models enable the integration of various types of georeferenced datasets, such as compositional, mineralogical, petrographic, structural, multi- and hyperspectral, geophysical, and petrophysical, across 1D, 2D, or 3D formats. However, manual interpretation of 3D point clouds remains labour-intensive, non-reproducible, and prone to human bias. Convolutional neural networks have been applied to segment the images used to build the 3D models, based on a few labelled training and testing subsets, to reduce the amount of human labour. This work used a U-Net encoder-decoder network architecture to segment images of sedimentary facies in reservoir analogue outcrop. The datasets vary in size from 500-1000 images with 40 MP resolution and in number of facies from 2-10. Different data processing pipelines were experimented with, including resizing and slicing due to memory constraints. Approximately 5-10 % of the images in each dataset were labelled by an expert interpreter, with half used for training and half for testing the model, yielding an overall accuracy of 70-85 %. The model was then retrained on the full labelled set and applied to the remaining unlabelled images. The final segmented outputs were processed through a photogrammetry pipeline to generate classified 3D point clouds, capturing the spatial distribution of architectural elements within the outcrop. This workflow allowed a reduction of 90% in manual labour with a high accuracy in the result.

How to cite: Gonçalves, Í., de Souza, E., Guadagnin, F., Roemers-Oliveira, E., Machado, E., Rangel, G., Freccia, A. C., Toledo, J., Schaffer, G., and Scherer, C.: Point cloud segmentation of sedimentary facies in outcrops with convolutional neural networks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8405, https://doi.org/10.5194/egusphere-egu26-8405, 2026.

The transition toward sustainable and resilient supply chains of critical minerals necessitates exploration workflows that are both data-intensive and methodologically transparent. Southeast Asia, which is located at the junction of three main metallogenetic domains, has huge potential for mineral exploration. However, in many ASEAN Member States, mineral exploration remains constrained by heterogeneous data quality, limited interoperability across survey systems, and insufficient integration of multi-scale observation modalities. To address these challenges, the Coordinating Committee for Geoscience Programmes in East and Southeast Asia (CCOP) and the Korea Institute of Geoscience and Mineral Resources (KIGAM) are jointly implementing the ASEAN-Korea Cooperation Fund project (2024-2026), aiming to advance capacity and infrastructure for technology-enabled, database-driven critical mineral exploration.

This contribution presents an integrated framework that couples field-scale acquisition systems with a data platform and a digital-twin-based 3D modeling exploration technology. The proposed workflow assimilates multi-source exploration datasets, including geological mapping, geochemical mapping, geophysical measurements, especially drone-based magnetic surveys, and in-situ terminals, into a unified digital representation of the subsurface. Within this digital twin paradigm, structural elements, geophysical inversion outputs, and associated attribute metadata are harmonized to support iterative model updating, uncertainty reduction, and reproducible interpretation of mineralization processes.

The platform implementation further emphasizes scalable database architecture, secure transmission and governance mechanisms, and interoperable interfaces to facilitate standardized data exchange and analysis. By extending conventional 2D GIS-based repositories toward a 3D exploration database with visualization and model-based analytics, the framework contributes to improved decision support for critical mineral exploration and underpins more robust mineral distribution databases aligned with principles of transparency and materiality commonly required for public reporting.

The CCOP–KIGAM-ASEAN regional collaboration demonstrates how digital-twin-based 3D modeling and integrated exploration data platforms can enhance analytical rigor, operational efficiency, and regional knowledge infrastructure for potential mineral exploration in ASEAN.

Keywords: Critical minerals; Mineral Exploration; Digital Twin; 3D Geological Modeling; Data Platform; ASEAN

How to cite: Wu, S. and Park, G.: Digital-Twin-Based 3D Geological Modeling and Integrated Exploration Data Platforms for Critical Mineral Exploration in ASEAN, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8578, https://doi.org/10.5194/egusphere-egu26-8578, 2026.

EGU26-8770 | Posters on site | ERE4.1

Development of a Bionic Self-Cleaning Drill Tool toward Enhanced In-Situ Fidelity in Subsea Sediment Sampling 

Pengyu Zhang, Wei Guo, Yuan Wang, and Rui Jia

Subsea sediment sampling is of great significance for marine geological research, resource exploration, environmental assessment, and geotechnical investigation. However, due to the common characteristics of high clay content, high water content, and under-consolidation of seabed sediments, conventional sampling techniques often cause severe sample disturbance, compression, or even loss. This leads to engineering challenges such as low core recovery and destruction of the original structure, which significantly compromises the in-situ characteristics and representativeness of the samples.Inspired by organisms (such as lotus leaves and earthworm) that maintain clean body surfaces in viscous environments, this study developed a material-structure coupled bionic anti-adhesion and drag-reduction surface by mimicking their micro-nano structure and low interfacial energy characteristics. This surface was constructed using a specific etching process combined with a low interfacial energy material coating technique and applied to the key contact parts of a subsea sediment sampling drill tool. Microstructural characterization and comparative sampling tests in typical clay and silty clay demonstrated that the bionic drill tool significantly reduces soil adhesion and frictional resistance during the sampling process. Consequently, it substantially increases the core recovery rate and effectively preserves the original stratigraphic sequence and moisture condition of the samples, markedly enhancing their in-situ fidelity.The bionic self-cleaning surface technology proposed in this study offers an innovative solution to the technical bottleneck of low-disturbance, high-fidelity sampling of highly viscous subsea sediments. Preliminary tests have verified the chemical stability and corrosion resistance of the surface coating in simulated seawater environments. Its long-term service reliability and large-scale engineering application processes require further research and optimization.

How to cite: Zhang, P., Guo, W., Wang, Y., and Jia, R.: Development of a Bionic Self-Cleaning Drill Tool toward Enhanced In-Situ Fidelity in Subsea Sediment Sampling, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8770, https://doi.org/10.5194/egusphere-egu26-8770, 2026.

Three-dimensional mineral prospectivity mapping (3D MPM) plays a key role in predicting deeply concealed mineral deposits; however, integrating heterogeneous datasets within machine learning frameworks remains a major source of uncertainty. In this study, we develop a gradient boosting ensemble method that explicitly adapts to different data representations and apply it to the Haopinggou gold polymetallic deposit in the western Henan metallogenic belt. Guided by mineral system theory and a 3D geological model, model performance and feature contributions are quantitatively evaluated using the SHAP framework. The results demonstrate that the binary-data-based gradient boosting model achieves higher AUC values and prediction accuracy than alternative approaches, and more effectively delineates deep exploration targets. These findings highlight the practical value of representation-aware ensemble learning for deep mineral exploration and target delineation.

How to cite: Fan, M., Xiao, K., Sun, L., and Xu, Y.: Three-Dimensional Mineral Prospectivity Mapping by a Gradient Boosting-Based Integrated Learning Method with Data Representation Adaptability, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-8798, https://doi.org/10.5194/egusphere-egu26-8798, 2026.

EGU26-9939 | ECS | Orals | ERE4.1

Towards robotic exploration without external infrastructure in underground mining environments: a case study from the PERSEPHONE project 

Christian Burlet, Nikos Stathoulopoulos, Vignesh Kottayam Viswanathan, Sumeet Gajanan Satpute, Giorgia Stasi, and George Nikolakopoulos

The PERSEPHONE Project supports the EU’s strategy to access deeper, previously abandoned or otherwise challenging underground mineral deposits in a more sustainable, safe and digitalised manner. In this context, the field deployment reported here at the Koutzi Mine (Evia, Greece) in September 2025 represents one of the demonstration missions of PERSEPHONE, during which a robotic platform performed mapping, relocalisation and multispectral mineral imaging without reliance on external infrastructure.

Robotic exploration of underground environments can serve not only as a means of new discovery, but also as a valuable tool for the remapping of historic galleries and more broadly for subterranean exploration (including caves and other naturally occurring voids). For instance, the UNEXMIN/UNEXUP projects have employed robotic systems to re-survey Europe’s abandoned flooded mines, as well natural flooded cavities like  the Molnár János cave (Hungary).

The geological setting of the Koutzi Mine is characterised by a narrow-vein magnesite deposit hosted in ophiolitic ultramafic lithologies on the island of Evia. This historic mine was reopened in 2021 and employs sub-level stoping with battery-operated excavators, reflecting a precision extraction philosophy designed to minimise environmental footprint. However, some of the older, smaller galleries remain unsafe for human exploration. The occurrence of magnesite (MgCO₃), frequently resulting from carbonation of ultramafic rocks, together with accessory white minerals such as sepiolite or opal in fault or alteration zones, provides a good target for multispectral imaging: determining vein type, thickness and mineral differentiation in this environment improves both exploration efficiency and robotics mission planning.

The exploration campaign comprised two phases. In the first phase, a agile mobile robot equipped with LiDAR and IMU sensors operated autonomously within the gallery, constructing a detailed volumetric map of several sections of the mine without use of GPS or pre-deployed reference beacons. Zones of interest were identified using the onboard visible-light camera to locate white-mineral zones. In the second phase, a second robot was introduced, successfully relocalized itself within the map created by the first robot and deployed to capture high-quality multispectral imaging of the identified white-mineral vein zones. The multispectral imaging subsystem comprised a near-infrared (NIR) camera and a UV-fluorescence camera mounted on the robot’s sensor suite. The objective was to acquire precise spectral–spatial data on vein geometries and white-mineral occurrences (distinguishing magnesite, sepiolite and opal) and to characterize thickness and orientation of the mineralized zones. By planning reference viewpoints with high overlap (80 %), the system links multispectral data with the 3D map context and supports subsequent data-driven analytics. Together with autonomous mapping and relocalization in absence of external infrastructure, this experiment provides a proof-of-concept of integrated robotic exploration, targeted mineral sensing and operational autonomy in an underground mining environment.

How to cite: Burlet, C., Stathoulopoulos, N., Viswanathan, V. K., Satpute, S. G., Stasi, G., and Nikolakopoulos, G.: Towards robotic exploration without external infrastructure in underground mining environments: a case study from the PERSEPHONE project, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9939, https://doi.org/10.5194/egusphere-egu26-9939, 2026.

EGU26-10886 | Posters on site | ERE4.1

Geospatial AI for Continuous Multi-Scale Risk Monitoring of Tailings Storage Facilities 

Feven Desta, Jan Růžička, Robin Bouvier, Louis Andreani, Lukáš Brodský, Martin Landa, Tomáš Bouček, Mike Buxton, Glen Nwaila, Mahsan Mahboob, Mulundumina Shimaponda, Mwansa Chabala, Cuthbert Casey Makondo, Laura Quijano, and Diego Diego Lozano

Tailings Storage Facilities (TSFs) represent one of the most critical and high-risk infrastructures in the mining sector, with failures leading to severe environmental, social, and economic consequences at local and transboundary scales. Increasing climate variability, ageing facilities, rising demand for mined products, and rising regulatory expectations necessitate more advanced TSF monitoring approaches.  Existing TSF monitoring is often fragmented, as Earth observation, in-situ sensing, and risk assessment tools operate independently, limiting their effectiveness for continuous risk assessment. This underscores  the need for integrated, multi-sensor monitoring approaches that can provide continuous, comprehensive, and predictive assessment of TSF stability and associated risks.
The GAIA-TSF (Geospatial Artificial Intelligence Analysis for Tailings Storage Facilities) project, led by an international consortium, aims to design and develop a prototype system. This system integrates satellite Earth Observation (EO) and ground-based sensor data with machine-learning (ML) algorithms to enable continuous, multi-level, and multi-scale characterization and monitoring of TSFs.
As a work in progress, the project has undertaken a comprehensive stakeholder engagement process to identify current gaps, operational needs, and priority monitoring requirements for TSFs. A review of the state of the art in available EO and ground-based monitoring technologies has been conducted, leading to the identification of key technologies and ML techniques. An extensive review of the literature, coupled with stakeholder input, led to the identification of key variables relevant to TSF monitoring. Such parameters include water quality, air quality, and slope stability. In parallel, potential test sites across different continents have been selected to support future calibration and validation of the prototype under diverse geographical and climatic conditions. The functional requirements and system architecture have been defined, identifying the key components of the prototype and how they are connected. The initial development phase of the GAIA-TSF prototype has commenced.
Integrated TSF monitoring supports risk-informed life-cycle management of TSF, enabling loss prevention and effective asset stewardship. It also strengthens decision-making for ESG compliance, the Global Industry Standard on Tailings Management (GISTM), and climate adaptation, ensuring safer and more sustainable mining operations.
The GAIA-TSF prototype offers a transferable and scalable continuous monitoring solution that enhances early anomaly detection and supports risk-informed decision-making. It thereby contributes to more sustainable and resilient TSF management.

How to cite: Desta, F., Růžička, J., Bouvier, R., Andreani, L., Brodský, L., Landa, M., Bouček, T., Buxton, M., Nwaila, G., Mahboob, M., Shimaponda, M., Chabala, M., Makondo, C. C., Quijano, L., and Diego Lozano, D.: Geospatial AI for Continuous Multi-Scale Risk Monitoring of Tailings Storage Facilities, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-10886, https://doi.org/10.5194/egusphere-egu26-10886, 2026.

EGU26-11149 | ECS | Orals | ERE4.1

A method for estimating the mineral contents from well logs using physics-informed neural networks 

Jiangbo Shu, Changchun Zou, and Cheng Peng

The composition contents of various minerals in the rock are a key concern in geophysical exploration and development. It is essential for lithology classification, the quantitative assessment of mineral resource potential, and reserves prediction. However, accurately calculating these mineral components is often highly challenging for formations with complex lithology, particularly when core samples and formation elemental logging data are scarce. In recent years, with the rapid development of artificial intelligence, utilizing big data and deep learning technologies to improve the accuracy and efficiency of well logging interpretation has become a research hotspot. Nevertheless, traditional data-driven models suffer from a lack of interpretability, which imposes certain limitations on their practical application. As a novel model integrating physical laws, Physics-Informed Neural Networks (PINNs) can constrain prediction results, rendering them more physically meaningful.

In this study, we propose a mineral content prediction model specifically designed for formations with complex mineral types. The model is capable of accurately calculating mineral contents using conventional logging data. First, based on the mineral types present in the formation, forward modeling is used to generate data and construct the training dataset. Subsequently, a CNN (Convolutional Neural Network) model is employed to predict the mineral content. By simultaneously constructing data loss and physical loss functions, the interpretability of the prediction results is ensured. The physical loss is mainly constructed by the volume model. The validity of the model is verified using forward modeling data. Finally, the model is applied to the processing of real logging data. The prediction results demonstrate good consistency with the mineral content obtained from X-ray Diffraction (XRD) analysis of core samples indicating that the model can accurately reflect the variations of complex mineral contents. This study provides a new method for the evaluation of mineral content, which is expected to offer a potential technological pathway for the identification of deep-seated ore bodies and the estimation of resource reserves.

This work is supported by National Science and Technology Major Project for Deep Earth Probe and Mineral Resources Exploration under Grant 2025ZD1008500.

How to cite: Shu, J., Zou, C., and Peng, C.: A method for estimating the mineral contents from well logs using physics-informed neural networks, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11149, https://doi.org/10.5194/egusphere-egu26-11149, 2026.

EGU26-12028 | ECS | Orals | ERE4.1

The antimony (Sb) resource in southern Tuscany (Italy): A multi-scale approach from textural and geochemical characterization to 3D geological modeling (Montauto mining area)   

Martina Rosa Galione, Pilario Costagliola, Pierfranco Lattanzi, Guia Morelli, Alessia Nannoni, Valentina Rimondi, Giovanni Ruggieri, Eugenio Trumpy, and Simone Vezzoni

Europe is highly dependent on foreign suppliers for several critical raw materials (CRMs), owing to limited domestic mining production. Antimony (Sb) has been included among Europe’s CRMs since the first list published in 2011, due to its extensive use in strategic industrial sectors. To meet the steadily increasing demand, new Sb orebodies must be identified, explored, and exploited within the European Union to diversify supply chains and reduce geopolitical risks. In parallel, the recovery of Sb from secondary sources, such as historical mining wastes, represents an additional opportunity.  

Within this framework, Italy has adopted the EU Critical Raw Materials Act, promoting the development of a national exploration plan. Antimony was historically mined in two Italian regions, Tuscany and Sardinia, leaving a substantial legacy of geological data (e.g., mining reports and drill logs) as well as significant volumes of mineral wastes. These Sb districts, where stibnite (Sb₂S₃) is the main economic mineral, represent an exceptional case study for assessing the potential Sb resources and associated CRMs in Italy. This study focuses on the Tuscan Sb district (e.g., the Mancianese area, southern Tuscany), where most of the available geological information is outdated and where robust constraints on orebody geometries, volumes, and associated CRM contents are still lacking (e.g., Lattanzi 1999). Here, we present the first results of an ongoing research project aimed at: 

  • Geological, mineralogical and geochimical data of Sb resources in Tuscany unravel ore genesis ;   
  • a 3D geological model of the selected orebodies, and potentially unexploited bodies, with probabilistic functions to conduct uncertainty analysis.  

Field surveys and sample collection were carried out in the Mancianese area and were integrated with textural analyses (reflected-light microscopy and SEM), mineral chemistry investigations (EPMA and LA-ICP-MS), stable and radiogenic isotope analyses and fluid inclusion studies. The collected dataset was used to reconstruct a 3D model of selected orebodies using GemPy, an open-source, Python-based geological modeling software. The results highlight the subsurface extent and continuity of mineralization, allowing a first-order estimate of the potentially available Sb resources. The resulting geological model not only contributes to the evaluation of the Italian Sb mining potential, which remains poorly constrained to date (SCRREEN, 2023), but also provides a robust framework for reconstructing the processes responsible for stibnite mineralization. This represents a valuable basis for future exploration and prospection campaigns in Southern Tuscany, offering essential knowledge for characterizing the mineral resource and developing genetic models that can also be applied to similar geological settings across Europe. 

How to cite: Galione, M. R., Costagliola, P., Lattanzi, P., Morelli, G., Nannoni, A., Rimondi, V., Ruggieri, G., Trumpy, E., and Vezzoni, S.: The antimony (Sb) resource in southern Tuscany (Italy): A multi-scale approach from textural and geochemical characterization to 3D geological modeling (Montauto mining area)  , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12028, https://doi.org/10.5194/egusphere-egu26-12028, 2026.

EGU26-12729 | Orals | ERE4.1

Rigorously quantifying observational uncertainty is essential for accelerating and automating geophysical inversions for subsurface mineral exploration 

Tom Hudson, Nick Smith, Martin Gal, Andrej Bona, Jan Hansen, Tim Jones, and Gerrit Olivier

The green energy transition is driving unprecedented demand for critical minerals. To meet this demand, we not only need to discover more mineral deposits, but accelerate the rate of these new discoveries. It is unlikely that many new discoveries will be based on surface observations alone, so geophysics will be valuable in providing the subsurface information required to find new deposits. However, applying geophysics to explore for new mineral deposits is limited by two key factors: uncertainty in subsurface images caused by non-uniqueness and the time taken to get these results from the field to decision makers. Better observational uncertainty quantification can address both these challenges. Here, we first emphasise the theoretical trade-off between subjective inversion choices and observational uncertainty, before practically showing the sensitivity of subsurface models output from geophysical inversions to observational (measurement) uncertainties via real-world examples. We first use an induced polarisation inversion to demonstrate how quantifying observational uncertainties not only results in more plausible subsurface images but also results that are less sensitive to subjective regularisation choices (due to decreased non-uniqueness). We then show a similar result for a seismology example: ambient noise tomography. We also briefly introduce the benefits for performing joint inversions and increasing inversion computational efficiency, as well as recent instrumentation advances that could drive a step-change in observational uncertainty quantification. The theoretical basis of what we show is not novel and the effects of quantifying observational uncertainty on output models are obvious. However, what we wish to emphasise here is instead the impact of quantifying uncertainty and rigorously including it in inversion workflows on reducing subjectivity of geophysical inversions. Reducing subjectivity is essential in the endeavour to automate inversion workflows. The drive to automate workflows is motivated by speed gains and near real-time exploration. If one can speed up inversion workflows then one can unlock near-real-time mineral exploration, allowing the mining industry to explore regions far faster than otherwise possible and meet the increased demand posed by the green energy transition.

How to cite: Hudson, T., Smith, N., Gal, M., Bona, A., Hansen, J., Jones, T., and Olivier, G.: Rigorously quantifying observational uncertainty is essential for accelerating and automating geophysical inversions for subsurface mineral exploration, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-12729, https://doi.org/10.5194/egusphere-egu26-12729, 2026.

EGU26-13973 | ECS | Posters on site | ERE4.1 | Highlight

EuroMineNet: Continuous Multitemporal Monitoring of Mining Dynamics in the European Union 

Weikang Yu, Vincent Nwazelibe, Xiaokang Zhang, Xiaoxiang Zhu, Richard Gloaguen, and Pedram Ghamisi

Mining activities are essential for the global energy transition, but they remain major drivers of land surface transformation and environmental degradation. Reliable, scalable monitoring of mining-induced land-use change is therefore critical for sustainable resource governance. In our earlier work, MineNetCD (2024) established the first global benchmark for mining change detection, enabling the identification of abrupt mining footprint changes from high-resolution bi-temporal imagery across 100 geographically diverse sites. While this provided a robust foundation for static change detection, sustainable mining oversight requires tracking the continuous and often gradual evolution of mining activities over time.

To address this limitation, we introduce EuroMineNet (2025), the first comprehensive multi-temporal mining benchmark designed for dynamic monitoring across the European Union. Leveraging a decade of Sentinel-2 multispectral imagery (2015–2024), EuroMineNet provides annual observations for 133 mining sites, enabling systematic analysis of both short-term operational dynamics and long-term land-use transformations.

The dataset supports two complementary, sustainability-oriented tasks: (1) Multi-temporal mining footprint mapping, producing temporally consistent annual delineations; and (2) Cross-temporal change detection, capturing gradual expansion, reclamation, and episodic disturbances.

To assess temporal consistency under evolving conditions, we propose a novel Change-Aware Temporal IoU (CA-TIoU) metric. Benchmarking 20 state-of-the-art deep learning models reveals that while current GeoAI methods perform well for long-term changes, they struggle with short-term dynamics crucial for early warning and mitigation. By advancing from global static detection to regional continuous monitoring, this work directly supports the European Green Deal and contributes to the development of transparent and explainable GeoAI tools for environmental resilience.

How to cite: Yu, W., Nwazelibe, V., Zhang, X., Zhu, X., Gloaguen, R., and Ghamisi, P.: EuroMineNet: Continuous Multitemporal Monitoring of Mining Dynamics in the European Union, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-13973, https://doi.org/10.5194/egusphere-egu26-13973, 2026.

EGU26-16870 | Posters on site | ERE4.1

 Adaptive LIBS analysis for estimating concentrations of alloy elements in heterogeneous metal scrap recycling streams  

Margret Fuchs, Aastha Singh, Rahul Patil, Mody Oury Barry, Gopi Regulan, Yuleika Carolina Madriz Diaz, and Richard Gloaguen

Metal scraps pose an economic and ecologically viable source for secondary resource supply to our industries, which call for more independence from global crises and strategic uncertainties. Well advanced technologies exist for steel and aluminum based on mechanical sorting using basic physical properties in order to split the major Fe- and Al rich fractions. However, many high-tech products require a precise composition specified by narrow acceptable ranges of alloy elements to achieve distint performances of a given alloy type. Here, traditional recycling stream processing bears limitations due to the generation of sorting fractions that contain mixes of variable alloy types, both, in steel as well as aluminum sorting products. Metallurgical processing of such mixed alloys, especially mixed aluminum alloys, leads to lower quality metals with less defined performance specifications and hence, the material is then lost for high-tech industries as a secondary resource. A more detailed, quantitative identification of specific alloy elements provides a solution, which allows for the differentiation between and consequent separation of alloy types. Here, laser-induced breakdown spectroscopy (LIBS) has shown enormous potential for trace (alloy) element detection. The remaining challenge or limitation lies in the strong matrix dependence of LIBS. This means, that a well pre-defined and homogeneous material stream is required for the accurate application of LIBS for element quantification and associated alloy identification.

We propose a hierarchical system to adapt LIBS analysis in a flexible way to the requirements of heterogeneous scrap recycling streams. We developed a clustering method to first identify the metal type, steel or aluminum, in mixed recycling products. The identified metal type provides the information on matrix conditions. Using then the respective calibration model for this matrix condition allows estimating precise alloy element concentrations in order to identify the alloy type. In repetition experiments, we could document high accuracies and precisions for specific diagnostic alloy elements, while few others show medium accuracies and precisions. The complementary information of elemental concentrations provides solid ground for an improved alloy detection and strategically points towards further options for dynamic thresholds in scrap processing procedures.

How to cite: Fuchs, M., Singh, A., Patil, R., Barry, M. O., Regulan, G., Madriz Diaz, Y. C., and Gloaguen, R.:  Adaptive LIBS analysis for estimating concentrations of alloy elements in heterogeneous metal scrap recycling streams , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-16870, https://doi.org/10.5194/egusphere-egu26-16870, 2026.

EGU26-17036 | Orals | ERE4.1

Advanced Geostatistical Models for Robust Mineral Resources Estimation in Complex Geological Settings 

Emmanouil Varouchakis, Maria Chrysanthi, Maria Koltsidopoulou, and Andrew Pavlides

Modern mineral exploration and production increasingly rely on advanced spatial modeling techniques capable of handling complex geological settings characterized by structural discontinuities, irregular sampling, and physical barriers. Conventional covariance models based on Euclidean distance measures often fail to adequately represent such environments, limiting their effectiveness in resource estimation and uncertainty quantification. The adoption of non-Euclidean distance metrics offers a promising pathway toward more realistic geological modeling and improved decision-making in mining operations.

This contribution presents recent advances in geostatistical covariance modeling based on the Linearly Damped Harmonic Oscillator, implemented through the Harmonic Covariance Estimator (HCE) and the Advanced Harmonic Covariance Estimator (AHCE). Nine case studies are used to demonstrate the applicability and robustness of these models across a broad range of mining-related scenarios, including univariate and multivariate mineral datasets, anisotropic orebody structures, unevenly distributed sampling, conditional simulations for uncertainty assessment and Gaussian anamorphosis models. Comparisons are made against established covariance models commonly used in mining geostatistics under both Euclidean and non-Euclidean distance frameworks.

Model performance is evaluated using leave-one-out cross-validation and eigenvalue-based validity testing. Results show that harmonic covariance models remain mathematically valid and predictive in complex geological environments where traditional approaches often fail. These advances provide a flexible and reliable framework for next-generation mineral resource modeling, supporting more accurate exploration targeting, improved production planning, and sustainable resource management in the mining industry of tomorrow.

The research project is implemented in the framework of H.F.R.I call “Basic research Financing (Horizontal support of all Sciences)” under the National Recovery and Resilience Plan “Greece 2.0” funded by the European Union – NextGenerationEU (H.F.R.I. Project Number: 16537)

M. D. Koltsidopoulou, A. Pavlides, D. T. Hristopulos,  E. Α. Varouchakis, 2025, Enhancing Geostatistical Analysis of Natural Resources Data with Complex Spatial Formations through non-Euclidean Distances, Mathematical Geosciences, in print.

A. Pavlides, M. D. Koltsidopoulou, M. Chrysanthi, E. A. Varouchakis, 2025. A Kernel-Based Nonparametric Approach for Data Gaussian Anamorphosis, Mathematical Geosciences, https://doi.org/10.1007/s11004-025-10251-z

E.A. Varouchakis, M. D. Koltsidopoulou and A. Pavlides, 2025, Designing Robust Covariance Models for Geostatistical Applications, Stochastic Environmental Research and Risk Assessment, https://doi.org/10.1007/s00477-025-02982-6

How to cite: Varouchakis, E., Chrysanthi, M., Koltsidopoulou, M., and Pavlides, A.: Advanced Geostatistical Models for Robust Mineral Resources Estimation in Complex Geological Settings, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17036, https://doi.org/10.5194/egusphere-egu26-17036, 2026.

EGU26-19063 | Orals | ERE4.1

Earth Observations and Proximity Sensing Technologies: Safer, More Sustainable, More Efficient Mining 

Jari Joutsenvaara, Ossi Kotavaara, and Marko Paavola

Modern society depends on raw materials for construction and infrastructure, but also increasingly for batteries, renewable energy, electronics, and the broader green transition. At the same time, mining faces tightening environmental expectations, safety requirements, and rising operational costs. The challenge is clear: how can we produce the minerals Europe needs while improving safety, lowering environmental impacts, and strengthening public trust? This book addresses that question by presenting practical, tested solutions based on a new generation of sensing and data technologies spanning Earth observation (EO) satellites, drone-based measurements, GNSS positioning, and proximity (in situ) sensing.
The volume was initiated and is primarily built on results from the EU Horizon 2020 project GoldenEye, which advanced the use of innovative monitoring and characterisation technologies to support safer and more sustainable mineral operations. GoldenEye’s central idea is simple but powerful: mining can be measured, understood, and managed more intelligently when we integrate information across scales from satellites that view entire mining districts, to drones that deliver site-scale detail, to local sensors and positioning systems supporting real-time operations underground and in active pits. Together, these technologies create objective, repeatable evidence of change. They can detect subtle ground movements, monitor tailings stability, map mining activity, characterise rock and ore properties, track vegetation and land-use evolution, and support early warning for environmental risks.
Crucially, the book treats mining as a complete life-cycle system, not only as “exploration and extraction”. The approaches discussed apply from early mineral exploration and resource evaluation, through mine development and active production, and onwards to closure, post-closure monitoring, and even mine reuse. For exploration, EO and hyperspectral methods can improve mineral targeting and reduce the need for costly field campaigns in remote areas. During operations, high-resolution sensing and precise positioning enable more efficient workflows and better safety management. For closure and post-closure, satellite and drone-based monitoring support objective tracking of ground stability and ecosystem recovery, strengthening compliance, transparency, and community confidence.
The volume is grounded in real-world deployment and realistic constraints. It discusses not only what technologies can do, but also their strengths, limitations, and readiness for adoption. The latter includes the skills needed, regulatory integration, and how multi-source data can be translated into reliable decisions. Overall, the book serves as both an accessible introduction and a scientific reference: responsible mining is inseparable from better measurement, and the GoldenEye legacy shows how modern sensing can enable safer, more sustainable, and more transparent mineral production.

How to cite: Joutsenvaara, J., Kotavaara, O., and Paavola, M.: Earth Observations and Proximity Sensing Technologies: Safer, More Sustainable, More Efficient Mining, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19063, https://doi.org/10.5194/egusphere-egu26-19063, 2026.

EGU26-19088 | Orals | ERE4.1

Urban Mining in Luxembourg: Integrating Geology and Engineering for Reliable Recycled Aggregate Concrete 

Markus Schäfer, Natascha Kuhlmann, Tom Berna, Michél Bender, Robert Colbach, Jean Thein, Paul Schosseler, and Stefan Maas

Increasing urbanisation and stricter environmental regulations have significantly restricted the exploitation of new gravel quarries as well as the local extraction of natural hard rocks and cement raw materials (lime, marl, clay), posing major challenges for the resource-intensive construction sector. In response, urban mining is gaining importance as a key strategy for circular construction. While natural aggregates from primary quarries provide well-established and consistent quality for concrete production, recycled aggregates (RA) and alternative cement raw materials derived from construction and demolition waste exhibit highly variable performance, strongly governed by source material characteristics and processing routes.

Luxembourg offers a particularly relevant case study due to its pronounced geological diversity and building heritage. The country is divided into the Palaeozoic Eisleck in the north, dominated by schistose rocks affected by Variscan deformation, and the Mesozoic Guttland in the south, characterised by an alternation of sandstones, limestones, dolomites, and marls with limited tectonic overprint. Most of these lithologies were historically used as local building stones, particularly in rubble stone masonry, which was constructed up to the early 20th century. As limestone and marl quarries supplying the cement industry become increasingly depleted or impossible to expand, construction and demolition waste from decommissioned buildings is becoming a significant secondary raw material source.

RA obtained through urban mining originates from highly heterogeneous feedstocks, including demolished concrete, manufactured masonry units, and natural rubble stone masonry. The suitability of rubble stone masonry for structural recycled aggregate concrete (RAC) depends on geological origin, mineralogical composition, the amount and properties of adhering mortar, and potential chemical pre-contamination, particularly by sulphates and chlorides. Porosity and pore-size distribution govern water absorption, workability, and strength development, while mineralogical factors such as alkali–silica reactivity critically affect durability. In addition, the presence of potentially toxic constituents may further limit reuse options.

This contribution presents an integrated geological–engineering approach for the evaluation of locally sourced RA. A material matrix for systematic lithological classification is proposed, linking geological characteristics with processing requirements and concrete performance. Adapted treatment chains - including selective demolition, targeted pre-sorting, and controlled crushing and screening - are identified as essential to ensure consistent RA quality.

Within the regulatory framework of EN 206, EN 206/DNA-LU, and EN 12620, the study demonstrates that properly processed rubble stone masonry can serve as a technically robust and normatively compliant raw material for RAC, supporting sustainable resource management through urban mining.

How to cite: Schäfer, M., Kuhlmann, N., Berna, T., Bender, M., Colbach, R., Thein, J., Schosseler, P., and Maas, S.: Urban Mining in Luxembourg: Integrating Geology and Engineering for Reliable Recycled Aggregate Concrete, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19088, https://doi.org/10.5194/egusphere-egu26-19088, 2026.

EGU26-20287 | ECS | Orals | ERE4.1

Critical Raw Material Potential and Mineral System Structure of the Northeastern Estonian Basement: A Geochemical, Geostatistical, and Geophysical Review 

Juan David Solano Acosta, Sophie Graul, Alvar Soesoo, Tarmo All, and Johannes Vind

The northeastern Estonian Precambrian basement, encompassing the Tallinn, Alutaguse, and Jõhvi domains, forms part of the eastern sector of the Fennoscandian Shield. This crustal segment comprises Paleoproterozoic back-arc volcanic–sedimentary successions intruded by Svecofennian granitoids and metamorphosed to amphibolite–granulite facies. Its lithological architecture and metallogenic characteristics show strong affinities with established mineralised provinces of southern Finland and central Sweden, including the Orijärvi and Bergslagen districts.

In this study, more than 500 historical drill cores, together with associated legacy geophysical datasets, were reanalysed to re-evaluate the mineral and critical-metal potential of the NE Estonian basement. Base- and precious-metal anomalies (Cu–Zn–Pb; Au–Ag–As–Sb) are spatially associated with magnetite-bearing and sulphide–graphite gneisses. High-resolution MSCL-XYZ scanning of archived drill cores further reveals a range of multi-element associations indicative of diverse mineral systems, including Ni–Co–Cr, Mo–W–Bi, Sn–Zn–Cd, Cu–Ni, Nb–Y–P, and Au–Ag–As–Sb–Bi–W–Se–Sn. These signatures delineate previously unrecognised prospective intervals across all three basement domains.

A compositional geostatistical workflow was applied to historical whole-rock geochemical data to mitigate biases arising from heterogeneous sampling density and analytical variability. Exploratory analyses conducted on raw datasets were complemented by centred log-ratio (clr) transformation, which enhanced coherence in multivariate patterns. Clr-based spatial maps, principal component analysis, and heat-map visualisations significantly improved the reliability of regional-scale interpretations and reduced artefacts related to mismatched neighbouring datasets.

Lithological descriptions from historical drilling, often incomplete or inconsistent, were reinterpreted using major-element geochemistry, while trace-element data were reassigned within a refined Tallinn–Alutaguse–Jõhvi basement framework. Integration of these geochemical reclassifications with gravity and magnetic data constrains subsurface architecture and strengthens correlations with mineral systems recognised in the southern Svecofennian domain and the Bergslagen province.

Overall, the integrated geochemical, geostatistical, and geophysical approach provides an updated metallogenic framework for the NE Estonian basement and identifies new exploration targets for critical raw materials, supporting ongoing research within the Horizon Europe DEXPLORE programme.

How to cite: Solano Acosta, J. D., Graul, S., Soesoo, A., All, T., and Vind, J.: Critical Raw Material Potential and Mineral System Structure of the Northeastern Estonian Basement: A Geochemical, Geostatistical, and Geophysical Review, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20287, https://doi.org/10.5194/egusphere-egu26-20287, 2026.

EGU26-20552 | ECS | Orals | ERE4.1

From Space to Field: Multi-Scale Characterization of Sediment-Hosted Copper Deposits in the Alma Inlier, Western Anti-Atlas, Morocco 

Ilham M'hamdi Alaoui, Ahmed Akhssas, Anas Bahi, Stéphanie Gautier, Hassan Ibouh, Nour Eddine Berkat, Mohammed Boumehdi, Hicham Khebbi, and Younes Abouabila

The Anti-Atlas, one of the oldest mountain chains in Morocco, has undergone multiple orogenic events that shaped its complex geology, making it a major province of sediment-hosted copper deposits, particularly in its western part. This study adopts a multi-scale, interdisciplinary workflow combining high-resolution hyperspectral remote sensing (up to 5 m spatial resolution), field-based spectral validation, geochemical analyses, and airborne geophysical data to achieve a comprehensive characterization of mineralization processes. Regional mapping of structural lineaments and copper-related alteration zones guided field investigations and the sampling of both mineralized and non-mineralized facies, allowing constraints to be placed on the origin of mineralization. These surface observations were subsequently linked to subsurface architecture through airborne geophysical modelling of regional geological cross-sections derived from field data. The integrated interpretation of all datasets enabled the development of a coherent geodynamic model adapted to the Alma Inlier. Overall, the proposed approach enhances exploration efficiency, reduces uncertainty, and supports more sustainable mineral exploration strategies.

Keywords:  Western Anti-Atlas, copper deposits, Hyperspectral remote sensing, Geochemical and geophysical integration, Exploration

How to cite: M'hamdi Alaoui, I., Akhssas, A., Bahi, A., Gautier, S., Ibouh, H., Berkat, N. E., Boumehdi, M., Khebbi, H., and Abouabila, Y.: From Space to Field: Multi-Scale Characterization of Sediment-Hosted Copper Deposits in the Alma Inlier, Western Anti-Atlas, Morocco, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20552, https://doi.org/10.5194/egusphere-egu26-20552, 2026.

EGU26-21304 | Orals | ERE4.1

Physics-Informed Annotation for Learning-Based Hyperspectral Mineral Mapping 

Matthias Kahl and Martin Schodlock

The retrieval of drill cores is a costly component of mineral exploration. Improving the spatial overview of mineral abundances within a deposit can substantially reduce the need for drilling. We present an unsupervised, automated annotation strategy for pixel-wise mineral labeling in hyperspectral imagery of simple deposit styles. In this context, a simple deposit style refers to deposits with very low or no mineral transitions and predominantly homogeneous, dominant mineral occurrences.

The automated annotation is based on handcrafted, mineral- and deposit-specific normalized difference indices (NDI). The objective is to extract a large number of representative mineral spectra for each occurring mineral. These spectra are subsequently used as training data for a targeted hyperspectral neural network with positional encoding, which is expected to generalize better to more complex deposit styles.

As a first step, the normalized mineral indices were successfully learned by the network, achieving an F-score of 0.98. This result represents a promising step toward physics-informed, neural-network-based mineral classification in hyperspectral imagery.

How to cite: Kahl, M. and Schodlock, M.: Physics-Informed Annotation for Learning-Based Hyperspectral Mineral Mapping, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21304, https://doi.org/10.5194/egusphere-egu26-21304, 2026.

Porphyry Cu deposits host the majority of global Cu resources and high-grade hypogene porphyry Cu deposits are of particular interest to industry because of the reduced waste and energy consumption required in exploitation, leading to favorable economics and reduced environmental impact. Detailed core logging, combined with TESCAN TIMA mineral quantification at two globally significant, high hypogene Cu grade, supergiant porphyry deposits – Resolution, USA and Hugo Dummett North, Mongolia, indicate that the majority of the chalcopyrite±bornite-pyrite are intergrown with muscovite that overprints earlier potassic alteration assemblages containing biotite and/or K-feldspar. Copper grades increase with the intensity of muscovite overprinting on primary potassic assemblages supporting the link between high-grade Cu mineralization and phyllic alteration. Another zone of high-grade Cu mineralization occurs in the upper parts of the phyllic alteration zone and/or within later advanced argillic alteration, associated with high-sulfidation bornite±digenite±covellite±chalcocite-pyrite assemblages, that partly replace earlier chalcopyrite. These two high grade domains have comparable features in many other significant HGHP deposits (Chuquicamata, Rosario, MMH, Onto, Butte) – all strongly telescoped systems that host significant amounts of high-grade Cu mineralization in phyllic and/or advanced argillic alteration that overprint potassic alteration.

We suggest there are at least three reasons for the development of high-grade hypogene ore in telescoped porphyry systems: 1) rapid unroofing and exhumation can generate steep thermal gradients, promoting a rapid decrease in Cu solubility and efficient precipitation of sulfides; 2) the most significant permeability creation in porphyry systems often develops late – during rapid, syn-mineralization exhumation and magma doming stages – when the rock mass behaves in an increasingly brittle fashion; 3) telescoping during syn-mineralization exhumation leads to overprinting of early sulfide assemblages by late-stage acidic and oxidized hydrothermal fluids that remobilize and concentrate early Cu, leading to the precipitation of sulfides with high Cu/S ratios. We conclude that the coincidence of rapid exhumation and long-lived hydrothermal activity exerts a first order control on the formation of high-grade hypogene porphyry Cu mineralization, meanwhile some other factors (such as favorable host rocks, high density of veins and breccias) are potential to form an individual high-grade porphyry Cu deposit.

How to cite: Yang, C. and Wilkinson, J. J.: Formation of giant high-grade hypogene porphyry copper deposits during phyllic to advanced argillic alteration: textural evidence from automated SEM mapping, Resolution and Hugo Dummett North deposits, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-23164, https://doi.org/10.5194/egusphere-egu26-23164, 2026.

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