Presentation type:
NP – Nonlinear Processes in Geosciences

Tipping points (TPs) are usually understood as bifurcations due to a slow parameter shift in a bistable system, where the system's state is diffusing around a fixed point in an underlying climate potential. As the shape of the climate potential changes towards the bifurcation, universal early-warning signals (EWS) due to critical slowing down appear.

How reliable is it to transfer this conceptual view to high-level risk assessments of climate change? We set out to test the anatomy and predictability of TPs in the complex system of the global ocean circulation, where changes in ice melt is a control parameter. Several findings highlight the need for more realistic methods to address the risk of TP:

1. The critical threshold of the control parameter can be fuzzy due to sensitive dependence on initial conditions and rate of non-adiabatic forcing changes.

2. In this spatially extended system, there is a high degree of multistability. This leads to a multitude of critical thresholds and abrupt changes in deterministic variability, which can interfer with EWS stemming from noise-driven fluctuations.

3. The universality of EWS in the high-dimensional case is compromised in practise, which may be mitigated by deriving system-specific observables from the properties of an edge state related to the TP.

How to cite: Lohmann, J.: Anatomy and predictability of tipping points in the high-dimensional climate system , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21955, https://doi.org/10.5194/egusphere-egu25-21955, 2025.

EGU25-121 | ECS | Posters virtual | VPS19 | Highlight

A Novel Q-Switch Technique for  Borehole NMR Measurement 

Sihui Luo, Xin Li, Huiju Yu, Zhengduo Wang, Tianyu Xing, Zhihao Long, Cheng Che, Guangzhi Liao, and Lizhi Xiao

Nuclear Magnetic Resonance (NMR) is a crucial logging technique for the unconventional and complex reservoir evaluation. However, the echo spacing is always an issue of borehole NMR measurement, which limits the performance of NMR tools to acquire the short relaxation components.

In this abstract, we proposed a novel Q-Switch technique aiming at breaking through the limitation of dead-time of borehole NMR logging tool, and to achieve much shorter echo spacing. Instead of using resistors of larger resistance in parallel with the radio-frequency (RF) coil to reduce the active dead-time, an inductive coupling circuit was introduced to decrease the ringing-down time significantly after transmitting the RF pulses with high voltage. The Q-Switch circuit consists of inductive coupling coil, capacitors, resistors and active high-voltage MOSFETs. The ringing-down time of RF system was decreased by at least 10 times compared to the system without using proposed Q-switch scheme, leading to echo spacing lower to 0.3 ms under the condition with resonant frequency lower to 500 kHz.

Both simulations and experiments were in great agreements, validating the feasibility and efficiency of proposed Q-switch scheme, and proved to be promising in the borehole NMR applications.

How to cite: Luo, S., Li, X., Yu, H., Wang, Z., Xing, T., Long, Z., Che, C., Liao, G., and Xiao, L.: A Novel Q-Switch Technique for  Borehole NMR Measurement, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-121, https://doi.org/10.5194/egusphere-egu25-121, 2025.

EGU25-4077 | ECS | Posters virtual | VPS19

Multiscale model coupling for watershed-scale contaminant transport modeling from point sources in Savannah River Site 

Kazuyuki Sakuma, Haruko Wainwright, Zexuan Xu, Angelique Lawrence, and Pieter Hazenberg

Soil and groundwater contamination at some sites impacts downstream populations when contaminants migrate from groundwater to rivers. Predictive modeling is challenging since it is required to include detailed subsurface structure and groundwater flow models within the site, as well as watershed-scale models for large-scale transport. Now that climate change impacts are major concerns at many sites, it is important to have the capability to represent the water balance change and its impact on contaminant transport both at the site and watershed scale in a consistent manner. This study introduces a new simulation framework to couple a detailed 2D site/hillslope-scale groundwater model to the 3D watershed-scale model to describe contaminant transport from groundwater to river water within the catchment. Within the site, we estimate the contaminant discharges to the river from contaminant sources based on the Richards equation and advection-dispersion equation. The discharges are then applied as the boundary conditions to the watershed-scale model considering the width of the 2D site/hillslope-scale groundwater model and recharge rates for both models.

We demonstrate and validate our framework based on the tritium concentration datasets in surface water and groundwater collected at the Savannah River Site F-Area. Results show that the method can successfully reproduce the contaminant concentration time series in river water.

How to cite: Sakuma, K., Wainwright, H., Xu, Z., Lawrence, A., and Hazenberg, P.: Multiscale model coupling for watershed-scale contaminant transport modeling from point sources in Savannah River Site, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4077, https://doi.org/10.5194/egusphere-egu25-4077, 2025.

EGU25-4641 | Posters virtual | VPS19 | Highlight

Size distribution of elemental components in atmospheric particulates from a typical industrial and mining city of Central China 

Hongxia Liu, Jiaquan Zhang, Changlin Zhan, Shan Liu, Ting Liu, and Wensheng Xiao

As one of crucial factor in atmospheric particulate matter, elemental components exhibit distinct distribution features within different particle size ranges. Crustal elements (such as Al, Si, Fe, Ca, Mg) are primarily concentrated in coarse particulate matter, whereas elements originating from anthropogenic pollution sources (such as heavy metal elements including Pb, Zn, Cd, As, Cr) are more frequently distributed in fine particulate matter. Furthermore, some specific elements may also exhibit peak concentrations in particular particle size, which is closely related to their sources and formation processes. In recent years, there are still some challenges and deficiencies. Further research is needed on the particle size distribution characteristics of complex pollution sources (such as industrial emissions and traffic emissions). Additionally, there is a need to enhance the understanding of the transformation mechanisms and health effects of elemental components within particulate matter. This study selected a typical industrial and mining city to investigate particle size distribution characteristics of elemental components in atmospheric particulate matter. Anderson Eight-Stage Particulate Impactor Sampler was used to collect atmospheric particulate matter in the urban area of Huangshi during winter and summer. Nine particle size range samples were obtained spanning from 0 to 0.4 µm, 0.4 to 0.7 µm, 0.7 to 1.1 µm, 1.1 to 2.1 µm, 2.1 to 3.3 µm, 3.3 to 4.7 µm, 4.7 to 5.8 µm, 5.8 to 9.0 µm, and 9.0 to 10 µm. Energy Dispersive X-Ray Fluorescence Spectrometry (ED-XRF) was employed to determine the concentrations of 17 elemental components, including S, Cl, K, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Rb, Sb, Ba, and Pb. Elements Ca, S, Fe, K, Zn, Ba, and Pb were identified as the primary pollutants during the sampling period. All the elemental concentrations exhibited distinct seasonal variations, demonstrating higher levels in winter compared to summer. Each element demonstrated distinct particle size distribution characteristics with peak concentrations for most elements occurring in the 5.8 to 9.0 µm range and peaks for the remaining elements in the 0.4 to 1.1 µm range. The highest elemental concentrations in both summer and winter were mainly distributed in the 5.8 to 9.0 µm and 0.7 to 1.1 µm size ranges. In summer, most elemental concentrations were negatively correlated with relative humidity. However, in winter, there was no significant correlation with relative humidity. Rainfall had a certain scavenging effect on elements but was also influenced by other meteorological factors. Element S had the highest enrichment factor values in both summer and winter. Element Cl was highly enriched in finer particle size fractions in both seasons. Most elements were slightly enriched across all particle size fractions. Principal component analysis further identified the main sources as soil dust and wind-blown sand, coal combustion, vehicle exhaust emissions, biomass burning, mining and construction activities, and other pollution sources. These findings contribute to the formulation of effective pollution control measures and the protection of public health.

How to cite: Liu, H., Zhang, J., Zhan, C., Liu, S., Liu, T., and Xiao, W.: Size distribution of elemental components in atmospheric particulates from a typical industrial and mining city of Central China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4641, https://doi.org/10.5194/egusphere-egu25-4641, 2025.

EGU25-7004 | Posters virtual | VPS19

Industrial High Performance Computing Scalable and FAIR Workflow Opportunities for EO Operations Processing, Operations, and Archiving 

Caroline Ball, Mark Chang, James Cruise, Camille de Valk, and Venkatesh Kannan
The computational demands of Sentinel data processing, archiving, and dissemination require scalable, efficient, and innovative solutions. While cloud computing-based services currently address these needs, integrating High-Performance Computing (HPC) systems into specific workflows could unlock a new level of industrial-scale capabilities. These include reduced processing times, faster data turnaround, and lower CO2 emissions. Leveraging HPC as a service allows for optimized data storage and access, enabling long-term strategies that prioritize essential data products and enhance operational efficiency.
Next-generation Quantum Computing (QC) holds the potential to redefine Earth Observation (EO) workflows by offering breakthroughs in solving complex optimization problems. As an operational service, QC could deliver significant cost and energy savings, provided that workflows can be seamlessly adapted to quantum-compatible infrastructures.
This presentation focuses on the evolution of HPC and QC technologies from research-driven concepts to industrial solutions, highlighting their maturity and applicability as services. We will explore the tangible benefits, associated costs, and pathways to operationalize these technologies for Level-0 to Level-2 data processing, operations, and archiving in support of current and future Sentinel missions.  We examine, at a high level, how artificial intelligence (AI) can provide a solution to hybrid HPC-QC challenges for EO data processing.

How to cite: Ball, C., Chang, M., Cruise, J., de Valk, C., and Kannan, V.: Industrial High Performance Computing Scalable and FAIR Workflow Opportunities for EO Operations Processing, Operations, and Archiving, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7004, https://doi.org/10.5194/egusphere-egu25-7004, 2025.

Severe convection, including thunderstorms and related phenomena like flash flooding, hail, and strong winds, can have significant socioeconomic impacts. Nowcasting, which provides real-time, short-term predictions, is vital for issuing timely warnings to mitigate these impacts. Satellite imagery is essential for monitoring convection and offering accurate predictions of storm evolution, thereby enhancing early warning systems. Ensemble forecasting, which generates multiple potential scenarios, helps better quantify uncertainties in nowcasting. However, most ensemble forecasting methods are computationally intensive and typically do not incorporate satellite images directly. The Analog Ensemble (AnEn) method, a lower-cost ensemble approach, identifies similar past weather events based on forecast data. For a given time and location, the AnEn method identifies analogs from past model predictions that are similar to current forecast conditions. Then their associated observations are used as ensemble members. Despite its advantages, AnEn struggles with locality and is sensitive to the choice of similarity metrics. This study presents an improved AnEn system that replaces forecast archives with satellite images to identify analogs of convective conditions. The system utilizes pretrained deep learning algorithms (VGG16, Xception, and Inception-ResNet) to assess image similarity. The training dataset consists of daily convection satellite images from EUMETSAT for the period 2020-2023, and the domain covers 40°N to 20°S and -20°W to 4°E. The year 2024 is used for testing, with ERA5 reanalysis of total precipitation as the verification ground-state. For a present convection satellite image this image is encoded and compared to all past encoded images of the training period using different metrics. The most similar images to the current one are then selected and their associated ERA5 total precipitation reanalysis are considered the members or our ensemble. Preliminary results indicate an average maximum precipitation anomaly of 15 mm between the analog ensemble mean and the current reanalysis, showing that the proposed system offers promising improvements in short-term forecasting.

Key words: Convection; Ensemble Forecasting; Deep Learning; VGG; Xception; ResNet; Analog Ensemble; Morocco; Nowcasting; EUMETSAT; ERA5; Morocco; Satellite Images; Remote Sensing;

How to cite: Alaoui, B., Bounoun, C., and Bari, D.: Leveraging Pretrained Deep Learning Models to Extract Similarities for the Analog Ensemble Method Applied to Convection Satellite Imagery, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7258, https://doi.org/10.5194/egusphere-egu25-7258, 2025.

Amid global environmental degradation, understanding the spatiotemporal dynamics and trade-offs of ecosystem services (ESs) under varying land-use scenarios is critical for advancing the sustainable development of social–ecological systems. This study analyzed the Chaohu Lake Basin (CLB), focusing on four scenarios: natural development (ND), economic priority (ED), ecological protection (EP), and sustainable development (SD). Using the PLUS model and multi-objective genetic algorithm (MOGA), land-use changes for 2030 were simulated, and their effects on ESs were assessed quantitatively and qualitatively. The ND scenario led to significant declines in cropland (3.73%) and forest areas (0.18%), primarily due to construction land expansion. The EP scenario curbed construction land growth, promoted ecosystem recovery, and slightly increased cropland by 0.05%. The SD scenario achieved a balance between ecological and economic goals, maintaining relative stability in ES provision. Between 2010 and 2020, construction land expansion, mainly concentrated in central Hefei City, led to a marked decline in habitat quality (HQ) and landscape aesthetics (LA), whereas water yield (WY) and soil retention (SR) improved. K-means clustering analysis identified seven ecosystem service bundles (ESBs), revealing significant spatial heterogeneity. Bundles 4 through 7, concentrated in mountainous and water regions, offered high biodiversity maintenance and ecological regulation. In contrast, critical ES areas in the ND and ED scenarios faced significant encroachment, resulting in diminished ecological functions. The SD scenario effectively mitigated these impacts, maintaining stable ES provision and ESB distribution. This study highlights the profound effects of different land-use scenarios on ESs, offering insights into sustainable planning and ecological restoration strategies in the CLB and comparable regions.

How to cite: Jin, A.: Ecosystem Services Trade-Offs in the Chaohu Lake Basin Based on Land-Use Scenario Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7785, https://doi.org/10.5194/egusphere-egu25-7785, 2025.

EGU25-7921 | ECS | Posters virtual | VPS19

Integrating high-resolution satellite and multispectral drone Imagery for monitoring vegetation in the Chaschoc-Sejá lagoon system 

Jacob Nieto, Nelly Lucero Ramírez Serrato, Alejandro Romero Herrera, Candelario Peralta Carreta, Graciela Herrera Zamarrón, Mario Alberto Hernández Hernández, Guillermo de Jesús Hernández García, Selene Olea Olea, Erick Morales Casique, and Alejandra Cortez Silva

Seasonal ecosystems play a crucial role in environmental regulation and biodiversity by hosting complex ecological dynamics that vary with climatic conditions. The Chaschoc-Sejá wetlands are a key example of such systems in southeastern Mexico. The interaction between the lagoon system and the Usumacinta River is highly dynamic; during the rainy season, the lagoons increase in volume, reaching depths of 8 to 10 meters. However, the lagoons completely dry up during the dry season, leaving vegetation at the surface level. 

This project aims to analyze the dynamics of vegetation cover in this environment by comparing high-resolution satellite images (Planet, 3 m) and ortho-mosaics generated with a DJI Mavic 3 Multispectral drone (10 cm). By combining these datasets, we aim to improve our previous vegetation maps and obtain a more accurate and detailed assessment of the Chaschoc-Sejá Lagoon system. Understanding vegetation patterns at a larger scale during specific periods and the variations in plant life within the lagoon and along its shores is a key focus.

 

Data processing involved classifying vegetation cover and identifying seasonal changes using indices such as NDVI and NDWI. We also generated 3D models to estimate vegetation height. Results show that integrating both techniques significantly improves spatial resolution and temporal accuracy in monitoring these ecosystems. This study provides essential tools for managing seasonal systems and their conservation in the face of climatic and anthropogenic factors. This monitoring will aid in understanding vegetation status, identifying plant species, and contributing to managing and preserving the lagoon system.

How to cite: Nieto, J., Ramírez Serrato, N. L., Romero Herrera, A., Peralta Carreta, C., Herrera Zamarrón, G., Hernández Hernández, M. A., Hernández García, G. D. J., Olea Olea, S., Morales Casique, E., and Cortez Silva, A.: Integrating high-resolution satellite and multispectral drone Imagery for monitoring vegetation in the Chaschoc-Sejá lagoon system, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7921, https://doi.org/10.5194/egusphere-egu25-7921, 2025.

Benevento Province, located in the Campania region of Italy, may experience environmental quality impacts from neighboring developed areas such as Naples and Caserta. Previous studies have suggested that some agricultural chemicals from Naples, such as hexachlorobenzene, may be transported through the air to rural areas of Benevento. Additionally, high concentrations of polycyclic aromatic hydrocarbons (PAHs) have been detected in Naples and Caserta, making Benevento Province a potential PAH "sink." This study systematically investigated the occurrence of PAHs in soil from Benevento Province, southern Italy, and their correlations with environmental factors, soil-air exchange processes, and health risks. Over 95% of sampling sites exhibited ∑16PAHs concentrations at non-polluted levels (9.50-1188 ng/g, mean = 55.0 ± 152 ng/g), and four-ring PAHs were the dominant pollutants contributing to 28.3% of ∑16PAHs. The spatial distribution of PAHs presented significant heterogeneity, with hotspots concentrated near landfills. The results of Positive Matrix Factorization (PMF) model showed that the main sources of PAHs were vehicle emissions, coal/biomass combustion, and petroleum products volatilization/leakage, contributing 42.2%, 40.2%, and 17.6%, respectively. Most of PAHs correlated significantly with total organic carbon in the soil and population density, while only Benzo(b)fluoranthene (BbF) showed a significantly negative correlation with pH. The mass inventory of ∑16PAHs ranged from 0.94 to 29.4 tons, averaging 2.45 tons. The synergistic effects of pollution hotspots and the persistent accumulation of PAHs in the soil suggested that the soil might act as a secondary source of PAHs. Toxicity equivalent and probabilistic risk assessments indicated that health risks from PAHs remained within acceptable limits.

How to cite: Qu, C. and Pu, C.: Investigation of polycyclic aromatic hydrocarbons in the soils of Benevento Province, Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10723, https://doi.org/10.5194/egusphere-egu25-10723, 2025.

EGU25-13330 | ECS | Posters virtual | VPS19

Advancing and Supporting FAIR Principle Adoption through Innovative Social Infrastructure Tools 

Leonie Raijmakers, Edvard Hübinette, Elianna DeSota, Sina Iman, and Philipp Koellinger

The adoption of the FAIR data principles has revolutionised data management in Earth System Sciences (ESS), yet challenges persist in achieving true machine-actionability and comprehensive implementation. 

DeSci Labs introduces two innovative tools—Decentralised Persistent Identifiers (DPIDs) and the CODEX protocol—to address the barriers to FAIR data practice implementation in general; whilst fostering widespread uptake of FAIR principles in the ESS community in particular through involvement in the FAIR2Adapt consortium.

DPIDs are globally unique persistent identifiers based on, and linked directly to, the content of the files it refers to. Each version of every file, regardless of type, is automatically assigned a cryptographic fingerprint, ensuring deterministic resolution and transparent versioning. The DPID has been specifically designed to support FAIR digital research objects. The flexibility to alias DPIDs with existing systems (e.g., DOIs) and programmatic publishing capabilities via NodesLib enhances interoperability while preserving data sovereignty.

The CODEX protocol, an open scholarly infrastructure, further complements this by enabling the storage and retrieval of FAIR digital research objects via a decentralised peer-to-peer network (IPFS). This architecture allows multiple copies of the same content to be stored by different network participants using the same PID. By empowering researchers to collaborate within an open-state repository, the protocol minimises reliance on centralised actors, ensuring long-term accessibility, data integrity, and transparency. Its modular design facilitates diverse gateway applications, maximising participation and reducing barriers to entry.

These tools address core challenges in FAIR adoption by providing robust, scalable, and interoperable solutions tailored to the ESS community. By integrating DPIDs and CODEX into data workflows, researchers can enhance data reusability, improve the provenance of research outputs, and safeguard the collective scientific record. This presentation explores how these technologies can catalyse the next decade of FAIR data practices in ESS, fostering trust, reproducibility, and innovation.

How to cite: Raijmakers, L., Hübinette, E., DeSota, E., Iman, S., and Koellinger, P.: Advancing and Supporting FAIR Principle Adoption through Innovative Social Infrastructure Tools, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13330, https://doi.org/10.5194/egusphere-egu25-13330, 2025.

EGU25-13917 | ECS | Posters virtual | VPS19

Automated Mineral Grain Extraction for Geometallurgical Studies Using Segment Anything Model (SAM) and Core Scanning Techniques 

Yuanzhi Cai, Ryan Manton, and Morgan Williams

In mineral exploration and geometallurgical studies, accurately segmenting mineral grains from core scanning datasets may be used to predict metal recovery. This study introduces the application of the Segment Anything Model (SAM), a cutting-edge deep learning tool, to automate the segmentation and extraction of mineral grains from Laser-Induced Breakdown Spectroscopy (LIBS) and hyperspectral core scanning datasets. SAM demonstrates high efficiency and precision in identifying mineral grains, forming the foundation for downstream analyses, including the evaluation of mineral associations, grain size distribution, and other key geometallurgical metrics. Through case studies on pegmatite deposits, this research showcases the potential of SAM to address challenges posed by mineralogically complex ore. By enabling detailed mineralogical characterisation and advancing geometallurgical methods, SAM-based grain extraction presents a transformative tool for supporting sustainable and efficient mining practices.

How to cite: Cai, Y., Manton, R., and Williams, M.: Automated Mineral Grain Extraction for Geometallurgical Studies Using Segment Anything Model (SAM) and Core Scanning Techniques, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13917, https://doi.org/10.5194/egusphere-egu25-13917, 2025.

EGU25-14821 | ECS | Posters virtual | VPS19

Simulation of Monthly Global Sea Surface Temperature Data using Ensemble GAN Model 

Deepayan Chakraborty and Adway Mitra

Synthetic data has become an indispensable tool in climate science, offering extensive spatio-temporal
coverage to address data limitations in both current and future scenarios. Such synthetic data, derived
from climate simulation models, must exhibit statistical consistency with observational datasets to ensure
their utility. Among global climate simulation initiatives, the Coupled Model Intercomparison Project
Phase 6 (CMIP6) represents the latest and most comprehensive suite of General Circulation Models
(GCMs). However, the substantial High Performance Computing (HPC) resources required for these
physics-based models limit their accessibility to a broader research community. In response, genera-
tive machine learning models have emerged as a promising alternative for simulating climate data with
reduced computational demands.
This study introduces an ensemble model based on the Pix2Pix conditional Generative Adversarial
Network (cGAN) to generate high-resolution spatio-temporal maps of monthly global Sea Surface Tem-
perature (SST) with significantly lower computational cost and time. The proposed model comprises two
components: the GAN, which produces simulated SST climatology data , and the Predictor, which is
trained with the variability of the data that forecasts SST anomaly for the subsequent month using the
output data from the previous month. Both components contain the same architecture, but the training
processes are different. The predictor model can be fine-tuned with observed data for some epochs to
adopt its domain.
The ensemble model was calibrated with monthly SST observations from the COBE dataset as in-
put and output. The Empirical Orthogonal Functions (EOF) shows the model’s ability to simulate the
variabilty of the observed data. The model’s performance was evaluated using the temporal Pearson cor-
relation coefficient and mean squared error (MSE). Results demonstrate that the ensemble cGAN model
generates maps with statistical characteristics closely matching those of CMIP6 simulations and obser-
vations, achieving a mean temporal correlation coefficient around 0.5 and an MSE around 1.13 for both
cases.

How to cite: Chakraborty, D. and Mitra, A.: Simulation of Monthly Global Sea Surface Temperature Data using Ensemble GAN Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14821, https://doi.org/10.5194/egusphere-egu25-14821, 2025.

EGU25-14839 | ECS | Posters virtual | VPS19

Leveraging MAUNet for Bias Correction of TRMM Precipitation Estimates 

Sumanta Chandra Mishra Sharma and Adway Mitra

Deep neural networks have revolutionized various fields due to their remarkable adaptability, enabling them to address related tasks through retraining and transfer learning. These capabilities make them invaluable tools for diverse applications, including climate and hydrological modeling. In an earlier work (Mishra Sharma et al., 2024), we introduced a novel neural network architecture, the Max-Average U-Net (MAUNet), which leverages Max-Average Pooling to downscale gridded precipitation data to higher spatial resolutions. The model demonstrated significant improvements in resolving finer-scale precipitation features, making it well-suited for climate data applications.

In this study, we utilized the MAUNet architecture to tackle the critical task of bias correction in satellite-based precipitation estimates. Bias correction is essential for improving the reliability of precipitation data derived from satellite missions, which often exhibit systematic discrepancies compared to ground-based measurements. Specifically, we focused on correcting biases in precipitation estimates from the Tropical Rainfall Measuring Mission (TRMM) by calibrating them against high-resolution, ground-based gridded datasets from the India Meteorological Department (IMD).

Our experimental results reveal that MAUNet effectively reduces biases in TRMM precipitation estimates, achieving significantly improved agreement with ground truth data. This success is attributed to the model’s robust feature extraction and reconstruction capabilities, which enable it to learn and correct systematic errors in satellite data. The findings also highlight the potential of advanced neural network architectures in addressing bias correction challenges.

This work underscores the utility of deep learning architectures in precipitation modeling, contributing to broader goals of improving the spatial distribution of precipitation estimates. By bridging the gap between satellite observations and ground truth, the MAUNet model offers a comprehensive solution for enhancing precipitation datasets, with significant implications for climate research, hydrological studies, and policy planning.

How to cite: Mishra Sharma, S. C. and Mitra, A.: Leveraging MAUNet for Bias Correction of TRMM Precipitation Estimates, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14839, https://doi.org/10.5194/egusphere-egu25-14839, 2025.

EGU25-15216 | Posters virtual | VPS19

A relevant accessible and interoperable geotechnical data tool to support the landslide risk management 

Graziella Emanuela Scarcella, Luigi Aceto, and Giovanni Gullà

The rising frequency and severity of landslides, exacerbated by the effects of climate change and human development in unstable areas, call for effective risk management strategies. In this context, a systematic collection of all the available data regarding geotechnical aspects, in particular geomaterial parameters, results plays a crucial role, providing a decisive contribution to define strategies for sustainable landslide risk management.

In this work, we present the translation of a geotechnical database to the aims of the project Tech4You Innovation Ecosystem – Goal 1 - Pilot Project 1, useful to identify the typical landslide scenarios, to identify sufficient knowledge for the definition of the geotechnical model and geomaterials typing in similar geo-environmental contexts. The database contains the results of laboratory tests carried out in the past by researchers at CNR IRPI in Rende, relating to 11 sites in Calabria, of which 10 in the Province of Catanzaro and 1 in the Province of Vibo Valentia.  For each site, geotechnical characterisation data of the geomaterials, which represent a key cognitive element, were grouped by type of laboratory test (grain size, indices, Atterberg limits, oedometric, direct shear and triaxial tests). We uploaded these data to validate a tool, named GeoDataTech vers. 2.0, which is an update of a previous version. In particular, we have tested the correct functioning (display, query, extraction data) with a significant sample of data. GeoDataTech vers. 2.0 can manage 2399 laboratory tests to date: 61 oedometric tests, 636 grain size, 537 indices, 78 Atterberg limits, 454 specific gravity, 512 direct shear tests and 121 triaxial tests.

This tool will be available to a wide range of stakeholders (researchers, professionals, territorial administrations, public bodies and citizens) allowing us to acquire, interrogate, export data and to upload their own files to integrate them into the database of the tool, performing advanced analyses with reference to the typification of geomaterials. By enabling the sharing of such data between researchers, practitioners and public institutions, the geotechnical tool will contribute significantly to improving disaster prevention strategies, in particular with regard to the reduction of landslide risks, thereby responding to the growing demand for accessible and interoperable data networks that increase synergic interdisciplinary research on topics such as landslide hazard.

This work was funded by the Next Generation EU—Italian NRRP, Mission 4, Component 2, Investment 1.5, call for the creation and strengthening of ‘Innovation Ecosystems’, building ‘Territorial R&D Leaders’ (Directorial Decree n. 2021/3277)—project Tech4You—Technologies for climate change adaptation and quality of life improvement, n. ECS0000009. This work reflects only the authors' views and opinions, neither the Ministry for University and Research nor the European Commission can be considered responsible for them.

How to cite: Scarcella, G. E., Aceto, L., and Gullà, G.: A relevant accessible and interoperable geotechnical data tool to support the landslide risk management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15216, https://doi.org/10.5194/egusphere-egu25-15216, 2025.

EGU25-15381 | ECS | Posters virtual | VPS19

Prediction of landuse landcover using CA-Markov model for the valley regions of Manipur, India 

Maisnam Nongthouba, Bakimchandra Oinam, and Khwairakpam Sachidananda

Changes in land use and cover (LULC) serve as critical indicators of socioeconomic and environmental shifts induced by both natural and man-made factors. This assessment was carried out in the Imphal valley region to forecast changes in land use and land cover. In order to examine the spatiotemporal distributions of LULC, the LULC Classification was analysed using Landsat images from 2007, 2014, and 2017. The CA-Markov Chain model was used to simulate the future LULC for the year 2030 of Imphal valley region based on these the past LULCs. The model result showed that wetland herbaceous will decline by 3.3% and settlement area will expand by 28.71%. The Imphal city area is where the majority of the expanding settlement area is located. As a vital resource for future planning initiatives, this study suggests planners, environmentalists, and decision-makers to prioritise sustainable practices and make appropriate decisions for the sustainability of the region.

How to cite: Nongthouba, M., Oinam, B., and Sachidananda, K.: Prediction of landuse landcover using CA-Markov model for the valley regions of Manipur, India, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15381, https://doi.org/10.5194/egusphere-egu25-15381, 2025.

EGU25-16092 | Posters virtual | VPS19

Transforming GNSS Data into FAIR Digital Objects 

Carine Bruyninx, Anna Miglio, Andras Fabian, Juliette Legrand, Eric Pottiaux, and Fikri Bamahry

GNSS (Global Navigation Satellite System) data play a crucial role in both scientific research and practical applications. GNSS datasets are used to monitor atmospheric conditions, tectonic plate movements, and Earth deformation, providing valuable insights for geodetic and geophysical studies. Although widely accessible, GNSS data often lacks the necessary structure and metadata for effective reuse, particularly for data-driven research based on machine learning. To address these challenges, we applied the FAIR (Findable, Accessible, Interoperable, Reusable) data principles to GNSS RINEX observation files hosted by the EUREF Historical Data Centre (EUREF-HDC).

The EU action plan “Turning FAIR into Reality” introduced the concept of FAIR Digital Objects (FDOs), emphasizing the need for Persistent Identifiers (PIDs) and rich, standardized metadata to ensure data can be reliably found, accessed, utilized, and cited. Building on this foundation, we developed a multi-layered FDO structure centered on GNSS RINEX data. Given the established nature of the EUREF-HDC repository, we adapted the FDO concept by prioritizing structured metadata, followed by persistent identifiers and robust (meta)data access procedures.

To implement this approach, we designed the GNSS-DCAT-AP metadata schema, assigned PIDs to both data and metadata, and developed web services enabling humans and machines alike to seamless search, retrieve, and download (meta)data. The effectiveness of our solution was evaluated using the FAIRsFAIR Data Object Assessment Metrics, demonstrating a significant improvement in FAIR compliance.

This work showcases the feasibility of transforming GNSS RINEX data into FAIR Digital Objects and could provide a practical roadmap for other geospatial data repositories seeking alignment with FAIR principles.

How to cite: Bruyninx, C., Miglio, A., Fabian, A., Legrand, J., Pottiaux, E., and Bamahry, F.: Transforming GNSS Data into FAIR Digital Objects, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16092, https://doi.org/10.5194/egusphere-egu25-16092, 2025.

EGU25-16363 | ECS | Posters on site | GI2.4

Hybrid Machine Learning approach for Tropical Cyclones Detection 

Davide Donno, Gabriele Accarino, Donatello Elia, Enrico Scoccimarro, and Silvio Gualdi

Tropical Cyclones (TCs) are among the most impactful weather phenomena, with climate change intensifying their duration and strength, posing significant risks to ecosystems and human life. Accurate TC detection, encompassing localization and tracking of TC centers, has become a critical focus for the climate science community. 

Traditional methods often rely on subjective threshold tuning and might require several input variables, thus making the tracking computationally expensive. We propose a cost-effective hybrid Machine Learning (ML) approach consisting in splitting the TC detection into two separate sub-tasks: localization and tracking. The TC task localization is fully data-driven: multiple Deep Neural Networks (DNNs) architectures have been explored to localize TC centers using a different set of input fields related to the cyclo-genesis, aiming also at reducing the number of input drivers required for detection. A neighborhood matching algorithm is then applied to join previously localized TC center estimates into potential trajectories over time. 

We train the DNNs on 40 years of ERA5 reanalysis data and International Best Track Archive for Climate Stewardship (IBTrACS) records across the East and West North Pacific basins. The hybrid approach is then compared with four state-of-the-art deterministic trackers (namely OWZ, TRACK, CNRM and UZ), reporting comparable or even better results in terms of Probability of Detection and False Alarm Rate, additionally capturing the interannual variability and spatial distribution of TCs in the target domain. 

The resulting hybrid ML model represents the core component of a Digital Twin (DT) application implemented in the context of the EU-funded interTwin project.

How to cite: Donno, D., Accarino, G., Elia, D., Scoccimarro, E., and Gualdi, S.: Hybrid Machine Learning approach for Tropical Cyclones Detection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16363, https://doi.org/10.5194/egusphere-egu25-16363, 2025.

The STARS4Water project addresses the critical need to understand the impacts of climate change and anthropogenic activities on freshwater availability and ecosystem resilience at the river basin scale. By developing innovative data services and models tailored to stakeholder needs, the project will improve decision-making processes for sustainable water resource management. A distinctive feature of STARS4Water is its focus on co-creating solutions with local stakeholders using a living lab approach, ensuring that newly developed tools remain relevant and usable beyond the life of the project.

 

This extension of the original project—funded with a special grant from Unitatea Executivă pentru Finanțarea Învățământului Superior, a Cercetării, Dezvoltării și Inovării (UEFISCDI) from Romania—focuses on a detailed change detection analysis to monitor and quantify land cover transformations in the emblematic Danube Delta region. The objective is to assess how environmental and anthropogenic changes have influenced this ecologically significant wetland over several decades. To achieve this, a comprehensive database of multispectral satellite images from the Landsat archive, spanning from 1985 to 2023, will be constructed. The long-term dataset enables a detailed temporal analysis, important for detecting land cover dynamics over time.

 

The methodology involves several key phases: (1) data collection and preprocessing of Landsat satellite images to correct errors and align imagery for consistent comparative analysis; (2) sampling and training a deep learning model using convolutional neural network (CNN) architectures, to classify various land cover types; (3) performing land cover classification on the processed images using the trained model, followed by accuracy assessment; and (4) conducting a comprehensive change detection analysis to quantify and interpret the observed transformations in land use and land cover.

 

The results of this analysis will deliver important knowledge on the long-term dynamics of the Danube Delta landscape, highlighting critical changes with implications for biodiversity, water management and ecosystem services. This approach will support adaptive ecosystem management and contribute to the scientific understanding of climate-related and anthropogenic changes in fragile wetland ecosystems.

 

Acknowlegments

This work was supported by a grant of the Ministry of Research, Innovation and Digitization, CNCS/CCCDI - UEFISCDI, project number PN-IV-P8-8.1-PRE-HE-ORG-2023-0094, within PNCDI IV.

How to cite: Scrieciu, A. and Toma, A.: Monitoring Long-Term Land Cover Transformations in the Danube Delta using Landsat Satellite Imagery, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16549, https://doi.org/10.5194/egusphere-egu25-16549, 2025.

EGU25-16634 | Posters virtual | VPS19

Finetuning and Benchmarking an AI Foundation Model for Cloud Gap Imputation  

Tadie Birihan Medimem, Gabriele Padovani, Takuya Kurihana, Ankur Kumar, Farid Melgani, Valentine G Anantharaj, and Sandro Luigi Fiore

Abstract: Cloud cover poses a significant obstacle in harnessing multi-spectral satellite imagery for various earth observation applications including disaster response, land use and land cover mapping. To address this issue, this study investigates the potential of Prithvi WxC foundation model (Johannes Schmude et al., 2024), a deep learning architecture designed for weather and climate applications, to perform cloud gap imputation. By leveraging its ability to capture atmospheric dynamics and predict missing data, Prithvi WxC offers a promising solution.

The primary objective is to assess the accuracy and efficiency of Prithvi WxC in reconstructing cloudy pixels in Moderate Resolution Imaging Spectroradiometer (MODIS) surface reflectance; MOD09 (Eric Vermote, 2015). MOD09 data provides valuable information about earth surface, cloud cover and atmospheric conditions, which are instrumental in informing the Prithvi WxC model during the finetuning and imputation process.

This research evaluates the Prithvi WxC foundation model for cloud gap imputation applications and benchmarks its performance against other foundation models, such as Prithvi EO (Jakubik et al., 2023, 2024). The process begins with preprocessing the MOD09 dataset, filtering out missing and cloudy pixels to create clean visible patches, while real-world cloudy patches are used as masks. The preprocessed data is then resampled to align with the temporal and spatial resolution requirements of both the Prithvi WxC and Prithvi EO foundation models. Through rigorous fine-tuning strategies, these models learn to reconstruct the masked regions, effectively filling the gaps caused by cloud cover. Finally, the fine-tuned foundation models are benchmarked using quantitative metrics, such as the Structural Similarity Index Measure (SSIM) and Mean Absolute Error (MAE), complemented by qualitative visual analysis.

This research explores the potential of Prithvi WxC foundation model, pre-trained on extensive weather and climate data, to improve cloud gap imputation in satellite imagery, and subsequently benchmarks it against earth observation foundation models, such as Prithvi EO. Through this evaluation, we aim to enhance scientific understanding via multi-modality and sensor-independent approaches.

 References

Johannes Schmude, Sujit Roy, Will Trojak, Johannes Jakubik, Daniel Salles Civitarese, Shraddha Singh, Julian Kuehnert, Kumar Ankur, Aman Gupta, Christopher E Phillips, Romeo Kienzler, Daniela Szwarcman, Vishal Gaur, Rajat Shinde, Rohit Lal, Arlindo Da Sil: Prithvi WxC: Foundation Model for Weather and Climate." arXiv preprint arXiv:2409.13598, 2024.

C. Roger, E. F. Vermote, J. P. Ray: https://modis-land.gsfc.nasa.gov/pdf/MOD09_UserGuide_v1.4.pdf. NASA, MODIS Surface Reflectance User’s Guide, Collection 6, 2015.

Daniela Szwarcman, Sujit Roy, Paolo Fraccaro, Þorsteinn Elí Gíslason, Benedikt Blumenstiel, Rinki Ghosal, Pedro Henrique de Oliveira, Joao Lucas de Sousa Almeida, Rocco Sedona, Yanghui Kang, Srija Chakraborty, Sizhe Wang, Ankur Kumar, Myscon Truong, Denys: Prithvi-EO-2.0: A Versatile Multi-Temporal Foundation Model for Earth Observation Applications. https://arxiv.org/abs/2412.02732, 2024.

Johannes Jakubik, Sujit Roy, C. E. Phillips, Paolo Fraccaro, Denys Godwin, Bianca Zadrozny, Daniela Szwarcman, Carlos Gomes, Gabby Nyirjesy, Blair Edwards, Daiki Kimura, Naomi Simumba, Linsong Chu, S. Karthik Mukkavilli, Devyani Lambhate, Kamal Das, Ranji: Foundation Models for Generalist Geospatial Artificial Intelligence, 2023.

Eric Vermote: MOD09 MODIS/Terra L2 Surface Reflectance, 5-Min Swath 250m, 500m, and 1km. NASA LP DAAC., NASA GSFC and MODAPS SIPS, NASA, http://doi.org/10.5067/MODIS/MOD09.061, 2015.

How to cite: Medimem, T. B., Padovani, G., Kurihana, T., Kumar, A., Melgani, F., Anantharaj, V. G., and Fiore, S. L.: Finetuning and Benchmarking an AI Foundation Model for Cloud Gap Imputation , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16634, https://doi.org/10.5194/egusphere-egu25-16634, 2025.

EGU25-18822 | Posters virtual | VPS19

Visualizing a climate and disaster resilience taxonomy from research evidence: scaling and accelerating knowledge interoperability 

Sukaina Bharwani, Rosie Witton, Kate Williamson, and Ruth Butterfield

The urgency of the climate crisis and the need to accelerate learning and climate action requires that we build on previous knowledge, rather than replicating it. There is an abundance of knowledge on climate change adaptation and mitigation dispersed across websites, projects, platforms, and documents. There is either too much information that is not easily discoverable (sitting in silos) or it is too technical or complex, and not ‘usable’ or fit for purpose in terms (e.g. language or format). Both issues cause redundancy and sometimes replication of work, wasting resources. In the worst case, they can also cause unintended consequences such as maladaptation, or increased vulnerability. However, the issue is not a lack of information, but rather how to organise and connect such knowledge to allow people to discover what already exists and put it to effective use. As such, our goal is to make climate action knowledge findable, accessible, interoperable and reusable (FAIR) and reduce climate change knowledge silos. The recently awarded FAIR2Adapt Project aims to establish a comprehensive FAIR and open data framework for CCA and to demonstrate the impact of FAIR data on CCA strategies. By making CCA data FAIR, FAIR2Adapt will accelerate adaptation actions so that they are visible, understandable, and actionable for various purposes and different types of stakeholders. FAIR taxonomies are one approach to help tackle this issue by making climate change knowledge FAIR and by ensuring, that going forward, platforms have a way to make their knowledge FAIR and thus more reusable by the climate change community. 


The Climate Connectivity Hub and Taxonomy seek to visualize and connect online platform data (e.g. Cordis, Climate-ADAPT, weADAPT, PreventionWeb) to increase discoverability, interoperability and a shared understanding of the research results and their potential application in future policy, research and practice. It builds on past knowledge to scale up and accelerate climate action whilst also identifying key knowledge gaps. This presentation will show that: 1) taxonomies are useful supporting the interoperability of online climate knowledge and can usefully emerge from combined expert and machine learning of project results (e.g. Cordis); 2) shared vocabularies and different interpretations of language and terminology add value to project planning and implementation ; and, 3) the visualization of these elements for decision-makers, planners, researchers, policy makers, etc. can help to enable and scale accelerated climate action. 

How to cite: Bharwani, S., Witton, R., Williamson, K., and Butterfield, R.: Visualizing a climate and disaster resilience taxonomy from research evidence: scaling and accelerating knowledge interoperability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18822, https://doi.org/10.5194/egusphere-egu25-18822, 2025.

EGU25-18933 | Posters virtual | VPS19

Deep Learning-based Spatial-Spectral Analysis for Peatland Degradation characterization 

Harsha Vardhan Kaparthi and Alfonso Vitti

The study explores using advanced deep learning (DL) techniques for spatial-spectral analysis to detect and map peatland degradation at a granular level. Peatlands, vital carbon sinks in global ecosystems, face degradation threats that demand precise and scalable monitoring solutions. Our method combines convolutional neural networks (CNNs), fully convolutional networks (FCNs), and 3D CNNs to examine complex spatial-spectral patterns in SAR, multispectral, and hyperspectral sensor data (e.g., Sentinel-1, Sentinel-2, PRISMA) over the temperate peatland study area of the Monte Bondone region (Latitude: 46°00’48.6” N, Longitude: 11°03'14.6” E), covering an area of 40 hectares as shown in the figures.

CNNs capture spatial relationships between precipitation, temperature, vegetation, soil, and moisture, offering a detailed view of peatland composition. Using multi-dimensional, gridded data from meteorological stations and remote sensing images, CNNs identify patterns affecting peatland health. Fully Convolutional Networks (FCNs) help with spectral unmixing, isolating land cover components at the pixel level, which aids in detecting vegetation degradation and understanding ecosystem changes.

3D CNNs incorporate temporal data to classify Peatland landscapes into different degradation states. The model identifies changes over time, distinguishing between healthy, partially degraded, and fully degraded regions. Deep clustering models also classify peatland areas into degradation states, revealing trends without labeled data.

This deep learning framework supports accurate degradation mapping through spatial-spectral feature extraction, providing precise, pixel-level information to aid ecosystem management and conservation. It helps monitor peatland health and assess environmental changes across diverse landscapes.

How to cite: Kaparthi, H. V. and Vitti, A.: Deep Learning-based Spatial-Spectral Analysis for Peatland Degradation characterization, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18933, https://doi.org/10.5194/egusphere-egu25-18933, 2025.

EGU25-19489 | ECS | Posters virtual | VPS19

Model-Agnostic Meta-Learning for Data Integration Across Heterogeneous Hydrological Datasets 

Asma Slaimi and Michael Scriney

Integrating heterogeneous hydrological datasets remains a significant challenge in environmental modelling due to variations in feature spaces, data distributions, and temporal and spatial scales across sources. This study introduces a Model-Agnostic Meta-Learning (MAML) approach to address the challenge of integrating heterogeneous hydrological datasets, leveraging a collection of datasets compiled from diverse sources. These datasets, characterized by varying features, distributions, and temporal and spatial scales, provide an ideal basis for evaluating MAML's ability to handle real-world data heterogeneity.

MAML’s unique capability to learn shared representations across datasets with minimal feature overlap and significant variability allows it to effectively transfer knowledge between subsets, offering a flexible and scalable solution for integrating hydrological data with diverse characteristics.

The proposed approach trains a base model on one subset of the data while utilizing MAML's meta-learning capabilities to adapt and transfer knowledge to other subsets with differing feature distributions. To test the model's adaptability, we simulate scenarios with varying degrees of feature overlap. Model performance is assessed using metrics such as mean squared error (MSE), both before and after fine-tuning on unseen data subsets.

Preliminary results demonstrate that MAML effectively learns shared representations across datasets, achieving significant improvements in prediction accuracy. Fine-tuning further enhances the model's adaptability, particularly for datasets with minimal feature overlap. These findings highlight MAML's potential as a powerful and flexible tool for integrating and predicting across heterogeneous hydrological datasets.

This study bridges the gap between advanced meta-learning techniques and hydrological applications, providing new insights into scalable and adaptable data integration methods for environmental sciences.

Keywords: Model-Agnostic Meta-Learning, hydrological datasets, data integration, heterogeneous data, meta-learning, environmental modelling, machine learning. 

How to cite: Slaimi, A. and Scriney, M.: Model-Agnostic Meta-Learning for Data Integration Across Heterogeneous Hydrological Datasets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19489, https://doi.org/10.5194/egusphere-egu25-19489, 2025.

EGU25-20324 | ECS | Posters virtual | VPS19

Using Remote sensing and geographic information system for delineating suitable sites for artificial groundwater recharge: A multi-criteria decision-making approach. 

Rahma Fri, Andrea Scozzari, Souad Haida, Malika Kili, Lamia Erraoui, Jamal Chaou, Abdelaziz Mridekh, Lahcen Goumghar, and Bouabid El Mansouri

The semi-arid region of Deraa Oued Noun in Morocco faces significant challenges related to water scarcity, which greatly affects the availability of groundwater resources. With recurring droughts and periods of water shortage, it is imperative to address these challenges and implement effective measures for sustainable groundwater resource management. Artificial groundwater recharge has proven to be a viable solution for alleviating water scarcity issues. By capturing and storing excess water during periods of heavy precipitation or surface water availability, artificial recharge can replenish depleted aquifers and provide a reliable water source during drought periods. However, the success of recharge projects depends on identifying suitable sites that meet specific criteria and maximize the efficiency of the recharge process.

The identification of suitable sites for artificial groundwater recharge in Daraa Oued Noun, through the integration of remote sensing, GIS (Geographic Information System), and MCDM (Multi-Criteria Decision Making) techniques, offers a promising solution to address water scarcity challenges in the context of climate change. The proposed research project aims to provide valuable and spatially explicit information for strategic groundwater resource management.

 This study was conducted in the Deraa Oued Noun district, where water shortages have been observed over the years. The research utilized geology, soil, land use, stream data, and Sentinel-2 and DEM images to develop thematic layers, including lithogeology, soil, slope, lineament density, land use, stream density, and water surface. Additionally, data on the vadose zone thickness were incorporated to enhance the analysis.

By integrating GIS and image processing techniques, these thematic layers were utilized to prepare groundwater recharge maps of the area through a weighted overlay method on a GIS platform. The results revealed that artificial recharge potential was high in the northern and western parts of the study area.

By following a systematic and rigorous methodology, including data collection, remote sensing analysis, MCDM evaluation, and site validation, this project aims to contribute to the successful implementation of artificial recharge projects in the region. By maximizing the efficiency of the recharge method, these projects will help ensure sustainable water supply, mitigate the impacts of drought, and promote long-term water security in Derâa Oued Noun and similar semi-arid regions.

How to cite: Fri, R., Scozzari, A., Haida, S., Kili, M., Erraoui, L., Chaou, J., Mridekh, A., Goumghar, L., and El Mansouri, B.: Using Remote sensing and geographic information system for delineating suitable sites for artificial groundwater recharge: A multi-criteria decision-making approach., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20324, https://doi.org/10.5194/egusphere-egu25-20324, 2025.

EGU25-20616 | ECS | Posters virtual | VPS19

LUCIE: A Lightweight Uncoupled ClImate Emulator with long-term stability and physical consistency for O(1000)-member ensembles 

Haiwen Guan, Troy Arcomano, Ashesh Chattopadhyay, and Romit Maulik

We present LUCIE, a data-driven atmospheric emulator that remains stable during autoregressive inference for a thousand of years with minimal drifting climatology. LUCIE was trained using 9.5 years of coarse-resolution ERA5 data, incorporating 5 prognostic variables, 2 forcing variables, and one diagnostic variable (6-hourly total precipitation), all on a single A100 GPU over a two-hour period. LUCIE autoregressively predicts the prognostic variables and outputs the diagnostic variables similar to AllenAI’s ACE climate emulator. Unlike all the other state-of-the-art AI weather models, LUCIE is neither unstable nor does it produce hallucinations that result in unphysical drift of the emulated climate. The low computational requirements of LUCIE allow for rapid experimentation including the development of novel loss functions to reduce spectral bias and improve tails of the distributions. Furthermore, LUCIE does not impose true sea-surface temperature (SST) from a coupled numerical model to enforce the annual cycle in temperature. We demonstrate the long-term climatology obtained from LUCIE as well as subseasonal-to-seasonal scale prediction skills on the prognostic variables. LUCIE is capable of 6000 years of simulation per day on a single GPU, allowing for O(100)-ensemble members for quantifying model uncertainty for climate and ensemble weather prediction.

How to cite: Guan, H., Arcomano, T., Chattopadhyay, A., and Maulik, R.: LUCIE: A Lightweight Uncoupled ClImate Emulator with long-term stability and physical consistency for O(1000)-member ensembles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20616, https://doi.org/10.5194/egusphere-egu25-20616, 2025.

EGU25-21759 | Posters virtual | VPS19

Assessment of Atmospheric Pollen Presence in Urban Areas of Greece During CALIPSO Overpasses 

Archontoula Karageorgopoulou, Stathopoulos Christos, Georgiou Thanasis, Shang Χiaoxia, Pyrri Ioanna, Amiridis Vassilis, and Giannakaki Elina

Analysis of pollen events was conducted using Hirst-type volumetric samplers in Athens and Thessaloniki in combination with CALIPSO vertical aerosol profiles. While Hirst-type ‎[1] volumetric samplers are used to confirm and characterize pollen at ground level, the understanding of pollen vertical distribution and transport is still limited. The utilization of Light Detection and Ranging (LIDAR) for identifying different pollen types is increasingly prevalent, as the depolarization ratio is related to the shape of the pollen particles while other non-spherical particle types are absent ‎[2].
Samplers are situated on the buildings’ rooftops of the Physics and Biology Departments, in Athens and Thessaloniki, respectively. Following ‎[2], intense pollen events are considered when the pollen concentration exceeds 400 grains m-3 for a minimum of two hours each day.
CALIPSO provides unique vertical profile measurements of the Earth’s atmosphere on a global scale ‎[3], with the ability to distinguish between feature types (i.e., clouds vs. aerosol) and subtypes (i.e., marine, dust, clean continental). Only case studies where CALIPSO aerosol layers were classified as marine, dusty marine, dust, or polluted dust were analyzed.
Model simulations were used to exclude the presence of other depolarizing aerosol types. HYSPLIT (Hybrid Single-Particle Lagrangian Integrated Trajectory) was used to trace the origin of the air masses. The atmospheric model RAMS/ICLAMS (Regional Atmospheric Modeling System/Integrated Community Limited Area Modeling System) was selected to describe dust and sea-salt emissions and transport.
Mean values of lidar-derived optical properties inside the detected pollen layers are provided from CALIPSO data analysis. Specifically, there are three observed aerosol layers, one over Athens (12-3-2021) and two over Thessaloniki (2-3-2020, 10-4-2020). Particulate color ratios of 0.652 ± 0.194, 0.638 ± 0.362, and 0.456 ± 0.284, and depolarization ratios of 8.70 ± 6.26%, 28.30 ± 14.16%, and 8.96±6.87 % for 12-3-2021, 2-3-2020 and 10-4-2020, respectively, were misclassified by CALIPSO as marine-dusty marine, dust and polluted dust. The pollen analysis conducted on the 12th of March 2021 indicated that the dominant pollen types were 69% Pinaceae and 24% Cupressaceae. On the 2nd of March 2020, Cupressaceae accounted for 97% of the total pollen, while on the 10th of April 2020, Carpinus represented 76% and Platanus 15%. Consequently, during periods of intense pollen presence, CALIPSO vertical profiles and aerobiological monitoring techniques may be used synergistically to better characterize the atmospheric pollen layers.

Acknowledgements
The research work was supported by the Hellenic Foundation for Research and Innovation (H.F.R.I.) under the “Basic Research Financing (Horizontal support for all Sciences), National Recovery and Resilience Plan (Greece 2.0)” (Project Number: 015144).

[1] J. M. Hirst, Annals of Applied Biology 39, 157-293 (1952).
[2] X. Shang et al., Atmos. Chem. Phys. 20, 15323–15339 (2020).
[3] D. M. Winker et al, BAMS 91, 1211–1229 (2010).

How to cite: Karageorgopoulou, A., Christos, S., Thanasis, G., Χiaoxia, S., Ioanna, P., Vassilis, A., and Elina, G.: Assessment of Atmospheric Pollen Presence in Urban Areas of Greece During CALIPSO Overpasses, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21759, https://doi.org/10.5194/egusphere-egu25-21759, 2025.

EGU25-2237 | Posters virtual | VPS20

Assessment of GOCI-II satellite remote sensing products in Lake Taihu 

Min Zhao, Huaming Li, Hao Li, Xuan Zhang, Xiaosong Ding, and Fang Gong

The Geostationary Ocean Color Imager-II (GOCI-II), which was launched on February 19, 2020, offers an increased observation times within a day and finer spatial resolution than those of its predecessor, the Geostationary Ocean Color Imager (GOCI), which was launched in 2010. To ensure the reliability of GOCI-II data for practical applications, the accuracy of remote sensing products must be validated. In this study, we employed in situ data from Lake Taihu for validation. We assessed the accuracy of GOCI-II products, including the remote sensing reflectance inverted via two atmospheric correction algorithms (ultraviolet (UV) and near-infrared (NIR) atmospheric correction algorithms), as well as the chlorophyll a (Chl-a) concentration, total suspended matter (TSM) concentration, and phytoplankton absorption coefficient (aph). Our results revealed that the UV atmospheric correction algorithm provided a relatively higher accuracy in Lake Taihu, with average absolute percentage deviations (APDs) of the remote sensing reflectance across different bands of 25.17% (412 nm), 29.69% (443 nm), 22.27% (490 nm), 19.38% (555 nm), 36.83% (660 nm), and 33.0% (680 nm). Compared to the products generated using the NIR atmospheric correction algorithm, the derived Chl-a concentration, TSM concentration, and aph products from the UV algorithm showed improved accuracy, with APD values reduced by 16.92%, 3.32%, and 10.91%, respectively. When using UV correction, the 412 nm band performed better than the 380 nm band, likely due to the lower signal-to-noise ratio of the 380 nm band and smaller extrapolation errors when assuming a zero signal for the 412 nm band. Considering that the NIR algorithm is suitable for open ocean waters while the UV algorithm demonstrates higher accuracy in highly turbid environments, a combined UV-NIR atmospheric correction algorithm may be more suitable for addressing different types of water environments. Additionally, more suitable retrieval algorithms are needed to improve the accuracy of Chl-a concentration and aph in eutrophic waters.

How to cite: Zhao, M., Li, H., Li, H., Zhang, X., Ding, X., and Gong, F.: Assessment of GOCI-II satellite remote sensing products in Lake Taihu, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2237, https://doi.org/10.5194/egusphere-egu25-2237, 2025.

EGU25-4994 | ECS | Posters virtual | VPS20

bibliometric analysis of natural lakes and paleolakes origin of natural events 

Jamal Abbach, Said El Moussaoui, Hajar El Talibi, and Charaf Eddine Bouiss

This study explores studies on lakes and paleolakes originating from natural effects. The main objective is to perform a bibliometric analysis of research on naturally occurring lake environments worldwide, covering the period from 2014 to 2024. Data extracted from 1687 documents in the Scopus database were analyzed using VOSviewer software. The results reveal a strict trend towards a focus on geosciences and the environment, underlined by research. This study particularly highlights the relationships between authors, co-authors, keywords, and publishers of specialized journals in this research field, thus providing essential information to guide future research and to value the role of these geological environments, which are rare in the world, based on essentially multidisciplinary geoscience approaches.

How to cite: Abbach, J., El Moussaoui, S., El Talibi, H., and Bouiss, C. E.: bibliometric analysis of natural lakes and paleolakes origin of natural events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4994, https://doi.org/10.5194/egusphere-egu25-4994, 2025.

Rock masses are characterized by the complex hierarchical structures involving various scale levels. The deformation of rock masses is primarily controlled in weak structural layers between rocks, whereas the rock block can be regarded as a non-deformable block and can move as a whole. In consequence, a new dynamic phenomenon, namely the pendulum-type wave, has emerged, which is a kind of nonlinear displacement wave caused by the overall movement of relatively intact large-scale rock blocks. Aiming at the complex hierarchical structures of rock masses and low-frequency characteristics of pendulum-type waves, the blocky rock masses composed of granite blocks and rubber interlayers are simplified into the block-spring model and wave motion model. Based on Bloch theorem and d’Alembert’s principle, the dispersion relation and equations of motion of 1D blocky rock masses are determined. Research shows that with the increase of the rock size and geomechanical invariant, the initial frequency of the first attenuation zone gradually decreases, and only the low-frequency waves lower than that frequency can propagate in blocky rock masses, which reveals the mechanism of low-frequency characteristics of pendulum-type waves theoretically. The equivalent substitution for the two models and their errors are given, and the results show that the equivalent substitution of the two models is not universal and unconditional. Finally, the influence of hierarchical structures on the dispersion relation and dynamic response is further studied. The larger the stiffness ratio, or the higher the order of hierarchical structures, the smaller is the effect of ignoring the high-order hierarchical structures.

How to cite: Jiang, K. and Qi, C.: Research on dispersion relation and dynamic properties of pendulum‑type waves in 1D blocky rock masses with complex hierarchical structures, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5033, https://doi.org/10.5194/egusphere-egu25-5033, 2025.

EGU25-5359 | ECS | Posters virtual | VPS20

Innovating Coral Reef Mapping with Drones & NASA Fluid Lensing Technology in the Mariana Islands 

Jonelle Sayama and Keanno Fausto

Coral reefs in the Mariana Islands serve important roles for the islands’ ecology and economy, contributing to the region’s fisheries, tourism, coastal protection, education, and cultural histories. Despite their immense value, the resilience of these marine ecosystems is threatened by an array of climate-change induced stressors, including ocean acidification and coral bleaching. In response, a team from the University of Guam (UOG) launched a large-scale coral reef mapping campaign to monitor priority reef sites throughout the Mariana Islands using drone technology. The UOG team, consisting of researchers and remote pilots funded by the USGS, Pacific Islands Climate Adaptation Science Center, NASA Guam EPSCoR, and NASA Guam Space Grant, has been conducting drone-based missions to capture high-resolution imagery of priority coral reef sites across Guam and Saipan. Their efforts aim to gather aerial data of coral reefs in Micronesia, providing resource managers with essential information regarding response and recovery. Initially, the campaign used of NASA’s fluid lensing technology developed by Chirayath (2019) for coral reef mapping. This technology combines unmanned aerial systems (UAS), off-the-shelf technology, and machine learning algorithms to create detailed coral reef maps by filtering out distortions caused by light and ocean waves, resulting in clear, high-resolution imagery. In 2024, this process was augmented to employ a new methodology that strategically uses RGB sensors and low tides. This system allows the remote pilots to capture the areas and produce orthomosaic maps at much more efficient rates while maintaining high-resolution quality. By providing these datasets within a shorter turn-around time, local natural resource managers are able to get a timely snapshot of the coral reef sites – providing crucial data of the ecosystem’s health that can help inform conservation decisions. This presentation will outline the collaborative efforts between UOG and regional partners, demonstrating how drones and fluid lensing technology are innovating coral reef monitoring efforts. It will explore how the collected data can help local resource managers make informed decisions regarding coral reef management, showcase coral reefs to the general public, ultimately transforming how local communities can contribute to coral reef resilience.

How to cite: Sayama, J. and Fausto, K.: Innovating Coral Reef Mapping with Drones & NASA Fluid Lensing Technology in the Mariana Islands, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5359, https://doi.org/10.5194/egusphere-egu25-5359, 2025.

EGU25-6240 | ECS | Posters virtual | VPS20

Enhancing the use of Geoinformation technologies to assess the socioeconomic impacts of climate change in the Arctic: Insights from the EO-PERSIST Project 

Georgios-Nektarios Tselos, Spyridon E. Detsikas, Beata Kroszka, Patryk Grzybowski, and George P. Petropoulos

In today's changing climate, there is an urgent need to understand the adverse impacts of climate change on natural environments, infrastructures, and industries.Particularly permafrost regions in the Arctic are highly vulnerable to global warming, impacting both the environment and socioeconomic aspects. Thus, systematic monitoring of such environments, is of paramount significance. Advances in Geoinformation technologies, and in particular in Earth Observation (EO), cloud computing, GIS, web cartography create new opportunities and challenges for Arctic research examining the socioeconomic impact of climate change.The rapid advancements in EOin particular have led to an exponential increase in the volume of geospatial data that come from spaceborne EO sensors. This surge, combined with the fast developments in GIS and web cartography present significant challenges for effective management, access, and utilization by researchers, policymakers, and the public. Consequently, there is a growing need for advanced methodologies to organize, process, and deliver geospatial information that comes from EO satellites in an accessible and user-friendly manner.

Recognizing thepromising potential of geoinformation technologies, the European Union (EU) has funded several research projects that leverage advanced technologies such as geospatial databases and WebGIS platforms to streamline EO data handling and dissemination. One such project is EO-PERSIST (http://www.eo-persist.eu), which aims to create a collaborative research and innovation environment focusing on leveraging existing services, datasets, and emerging technologies to achieve a consistently updated ecosystem of EO-based datasets for permafrost applications. To formulate the socioeconomic indicators, the project exploits state of the art cloud processing resources, innovative Remote Sensing (RS) algorithms, Geographic Information Systems (GIS)-based models formulating, exchanging also multidisciplinary knowledge.EO-PERSIST innovative approach is anticipated to contribute to more informed decision-making and broader data accessibility for researchers, policymakers, and other stakeholders.

The present contribution aim is two-fold: at first, to provide an overview of EO-PERSIST Marie Curie Staff Exchanges EU-funded research project; second, to present some of the key project outputs delivered so far relevant to the selected Use Cases of the project and the geospatial database developed for assessing the socioeconomic impacts of climate change in the permafrost Arctic regions.

This study is supported by EO-PERSIST project which has received funding from the European Union's Horizon 2020 research and innovation program under grant agreement No. 101086386.

KEYWORDS:earth observation, cloud platform, Arctic, socioeconomic impact

How to cite: Tselos, G.-N., Detsikas, S. E., Kroszka, B., Grzybowski, P., and Petropoulos, G. P.: Enhancing the use of Geoinformation technologies to assess the socioeconomic impacts of climate change in the Arctic: Insights from the EO-PERSIST Project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6240, https://doi.org/10.5194/egusphere-egu25-6240, 2025.

EGU25-8063 | ECS | Posters virtual | VPS20

Deploying UAV technology to assess typhoon impacts in vulnerable communities in Guam  

Keanno Fausto and Jonelle Sayama

The U.S. territory of Guam is threatened annually by high-intensity storms and typhoons due to its location in the western Pacific Ocean. The island’s infrastructure – buildings, roads, and utilities – bear the brunt of typhoon damage, which in turn affects public health, the economy, and natural resources. Traditionally, these impacts have been observed via satellite, radar, and official weather stations.  Damages are assessed in the aftermath of the typhoon with a manual, on-the-ground approach led by the National Weather Service (NWS). This is often exhaustive and time-consuming for the assessment team. Observations from the ground can inadvertently create data gaps on damage assessments due to inaccessible areas caused by vegetative and construction debris, and flooded roads and pathways. This may not capture many impacts eligible for local or federal assistance. To address these data gaps and augment damage assessments, the University of Guam (UOG) Drone Corps program aims to assist local and federal government agencies (e.g., utility companies, public health, emergency services, and natural resource management) by collecting high-resolution aerial imagery to help prioritize and allocate limited resources. This presentation highlights the results of this novel collaboration of UOG, NWS, Guam Homeland Security (GHS), and the Office of the Governor of Guam in the creation of the damage assessment of Typhoon Mawar, which ravaged Guam on 24-25 May 2023. Following the typhoon, UOG worked with NWS to identify and capture imagery of vulnerable sites that were heavily impacted. This presentation will also share how UOG Drone Corps’ data was disseminated among other agencies as supplemental data for natural disaster recovery efforts. The presentation will conclude with a summary of the UOG Drone Corps program model as a resource for developing resiliency strategies for vulnerable island communities using advanced and emerging technologies. 

How to cite: Fausto, K. and Sayama, J.: Deploying UAV technology to assess typhoon impacts in vulnerable communities in Guam , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8063, https://doi.org/10.5194/egusphere-egu25-8063, 2025.

EGU25-11808 | ECS | Posters virtual | VPS20

The use of InSAR and DInSAR for detecting land subsidence in Albania 

Pietro Belba

INTRODUCTION. InSAR or Interferometric Synthetic Aperture Radar is a technique for mapping ground deformation using radar images of the Earth's surface collected from orbiting satellites. DInSAR or Differential SAR Interferometry is an active remote sensing technique based on the principle that, due to the very high stability of the satellite orbits, it is possible to exploit the informative contribution carried by the phase difference between two SAR images looking at the same scene from comparable geometries.

AIM. In this setting, the main objective of this study is to evaluate the region near the closed rock salt mine in the south of Albania. Our input for this exercise will be two images of the land near the former rock salt mine in Dhrovjan near the Blue Eye (Saranda, Albania).

RESULTS. By combining the phases of 2 images we produce an interferogram where the phase is correlated to the terrain topography and deformation so if the phase shifts related to the topography are removed from the interferogram, the difference between the resulting products will show surface deformation patterns or cure between the two acquisition dates and this methodology is called differential interferometry Processing, Phase Unwrapping, and at the end creating the displacement map. We use in our study the difference in time with the algorithm which consists of working step by step with these operators: Read the two split products, Applying Orbit files, Back-Geocoding, Enhanced Spectral Diversity, Interferogram, TOPSAR Deburst, and Write. The resulting difference of phases is called an interferogram containing all the information on relative geometry. Removing the topographic and orbital contributions may reveal ground movements along the line of sight between the radar and the target.

The next algorithm we worked with these operators: Read the debursted interferogram, TopoPhaseRemoval, Multilook, Goldstain Filtering, and Write. At the same time from Goldstain Filtering, we add the Snaphu Export operator.

Correct phase unwrapping procedures must be performed to retrieve the absolute phase value by adding multiples of 2π phase values to each pixel to extract accurate information from the signal. In this study, we will use SNAPHU, which is a two-dimensional phase unwrapping algorithm consists of working step by step with these operators: read (the wrapped image) and read (2) the unwrapped image, Snaphu Import, PhaseToDisplacement, and Write. We can display it in Google Earth after saving it as .kmz and also make a profile of the displacements.

DISCUSSION AND CONCLUSIONS

One of the SAR Interferometry applications is deformation mapping and change detection. This work demonstrates the capability of interferometric processing for the observation and analysis of instant relative surface deformations in the radar LOS direction. When two observations are made from the same location in space but at different times, the interferometric phase is proportional to any change in the range of a surface feature directly. All three stages of the work are important and require accurate interpretation knowledge, especially when working with the Snaphu program.

KEY-WORDS

InSAR, DInSAR, Interferogram

How to cite: Belba, P.: The use of InSAR and DInSAR for detecting land subsidence in Albania, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11808, https://doi.org/10.5194/egusphere-egu25-11808, 2025.

EGU25-12947 | ECS | Posters virtual | VPS20

Topological fingerprinting of dynamical systems 

Gisela Daniela Charó, Davide Faranda, Michael Ghil, and Denisse Sciamarella

Poincaré established a framework for understanding the dependence of a dynamical system's properties on its topology. Topological properties offer detailed insights into the fundamental mechanisms — stretching, squeezing, tearing, folding, and twisting — that govern the shaping of a dynamical system's flow in state space. These mechanisms serve as a conduit between the system's dynamics and its topology [Ghil & Sciamarella, NPG, 2023]. A topological analysis based on the templex approach [Charó et al., Chaos, 2022] involves finding a topological representation of the underlying structure of the flow by the construction of a cell complex that approximates its branched manifold and a directed graph on this complex. A pivotal feature of the cell complex that facilitates the characterization of the flow dynamics is the joining locus, upon which all the fundamental mechanisms that sculpt the flow leave a pronounced signature.

The local dimension d(x) and the inverse persistence θ(x) of the state x of a dynamical system [Lucarini et al., 2016; Faranda et al., Sci. Rep., 2017] provide information on the rarity and predictability of specific states, respectively. We demonstrate herein that these two measures, d and θ  also provide information about the localization of the joining locus.

The present work proposes a new topological method for fingerprinting a system’s nonlinear behavior using the concept of persistent generatexes. This novel approach integrates the strengths of two topological data analysis methods: the templex and persistent homologies. Rather than employing a single cell complex and a digraph to characterize the flow of the system, our approach emphasizes the localization of the joining locus through the calculation of local dimension and the inverse persistence, leading to the construction of a family of nested digraphs. The dynamical paths, namely the nonequivalent ways of travelling through the flow, are found to be the most persistent cycles; here the concept of persistence is used in the sense of the persistent homology approach [Edelsbrunner & Harer, Contemporary mathematics, 2008]. The dynamical paths give us the ‘topological fingerprinting’ of a system’s dynamics.

How to cite: Charó, G. D., Faranda, D., Ghil, M., and Sciamarella, D.: Topological fingerprinting of dynamical systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12947, https://doi.org/10.5194/egusphere-egu25-12947, 2025.

The Er-Rich region is a focal area for understanding the geological evolution of the central-eastern High Atlas, which it covers almost entirely along a north-south transverse line. It is a hinge region between the two major tectonic structures of the High Atlas (the North and South Atlas faults), which reveal a framework of Meso-Cenozoic carbonate, detrital and magmatic rocks.

Previous studies have highlighted the complexity of mapping in this area. To date, no detailed geological map has been produced for this study area, with the exception of the old provisional 1:200,000 map of the Midelt-Rich High Atlas. Remotely-sensed mapping initiatives have also been carried out in the region, except that they do not provide a final interpretation as a geological map, supported by geological maps covering neighboring regions. A detailed geological map of the Er-Rich region, based on the results of remote sensing and field data, is therefore needed in the area. For this purpose, remote sensing geological mapping techniques have been applied to two types of satellite data: 1) Landsat 8 OLI (Optical Land Imager) multispectral optical data, and the Spot 5 panchromatic band acquired by the HRG-2 (High Geometric Resolution) instrument; 2) Sentinel-1 SAR data with dual polarisation (HV-HH).

All the data underwent several pre-processing or correction stages using appropriate software, in particular radiometric and atmospheric correction for Landsat 8 OLI (Optical Land Imager) images using ENVI software. The corrected product of the three Landsat 8 OLI scenes covering the region were then spatially enhanced using the Spot 5 panchromatic band to produce a multispectral image with a high spatial resolution of 5 m using ENVI software. The Sentinel-1 radar data were pre-processed using SNAP toolbox software by applying a series of corrections.

The results obtained by applying the Optimum Index Factor (OIF) method and Principal Component Analysis (PCA), allowing us to select the most significant colored compositions. Moreover, this combination enabled us to delineate with great precision the large outcrops of carbonate rocks (limestones, marl), siliciclastic rocks (conglomerates, sandstones and silts) and magmatic rocks (igneous intrusions).

The lineaments were extracted manually by visual interpretation of Sentinel-1 radar images, after applying directional filtering folowing four general orientations (N0, N45, N90, N135), enabling us to generate a synthetic structural map of the region.

The results obtained were compared with data from geological maps of adjacent areas and approved by field observations, leading to the production of a high-precision geological map, compiled with pre-existing geological literature.

How to cite: Hdoufane, M., Zafaty, O., and Ettaki, M.: Integrated remote sensing data and field investigations for geological mapping and structural analysis in the Er-Rich area (High Atlas, Morocco), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13782, https://doi.org/10.5194/egusphere-egu25-13782, 2025.

EGU25-15569 | Posters virtual | VPS20

Uniform Data Access Layer: Advancing Data FAIRness in FAIR-EASE 

Jorge Mendes and Marc Portier

The Uniform Data Access Layer (UDAL), a central component within the FAIR-EASE project, is designed to revolutionize how researchers access, integrate, and utilize diverse scientific datasets. FAIR-EASE prioritizes FAIR (Findable, Accessible, Interoperable, Reusable) principles to ensure that data becomes a powerful enabler of scientific discovery and informed decision-making. 

The UDAL concept brings a modular and re-usable approach to choosing and using data in data processing workflows. It materializes as a software package that users can use in their pipelines. UDAL serves as a middleware layer, offering a standardized, user-centric framework for data access. By bridging the gap between complex infrastructures and researchers, UDAL simplifies data retrieval, integration, and usage. This solution decouples data usage from technical complexities, ensuring that researchers can focus on analysis without needing detailed knowledge of access protocols or data formats. Its adaptability to a wide range of technologies and protocols enables interoperability across disciplines and geographic regions. UDAL's innovative approach has been validated with data providers such as Argo and Blue-Cloud and various technology stacks and formats like NetCDF, Beacon, SPARQL endpoint, HTTP REST API, demonstrating its capacity to unify diverse datasets into a single, intuitive system. 

A key feature of UDAL is its "named query" mechanism, which standardizes and reuses specific data requests. This enhances reproducibility, shields users from the intricacies of data filtering and retrieval, and promotes efficiency. Additionally, UDAL’s technology-agnostic approach accommodates centralized and distributed data architectures, supporting innovation in data management and usage strategies. 

By addressing critical challenges in data management—such as technical barriers and the diversity of data sources—UDAL aligns with the broader goals of FAIR-EASE. It empowers both researchers and data providers, fostering cross-domain collaboration and innovation. Beyond its technical contributions, UDAL embodies a vision of “data as a commodity,” promoting the sustainability and accessibility necessary for open science. While it does not directly address equitable benefit distribution, its transparent usage measurement capabilities lay a foundation for future policy and governance frameworks. 

In conclusion, UDAL represents a transformative advance in data-driven research, harmonizing access across disciplines and platforms while accelerating discovery and fostering innovation. As a cornerstone of FAIR-EASE, UDAL is set to establish new standards for simplicity, usability, and sustainability in scientific data management. 

How to cite: Mendes, J. and Portier, M.: Uniform Data Access Layer: Advancing Data FAIRness in FAIR-EASE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15569, https://doi.org/10.5194/egusphere-egu25-15569, 2025.

EGU25-16203 | ECS | Posters virtual | VPS20

Temporal and Spatial Dynamics of Urban Evapotranspiration in Paris: A Multiscale Perspective 

Sitian Zhu, Auguste Gires, Daniel Schertzer, Ioulia Tchiguirinskaia, and Cedo Maksimovic

The impacts of global change, such as extreme heat and water scarcity, are increasingly threatening urban populations. Evapotranspiration (ET) plays a vital role in mitigating urban heat islands and reducing the effects of heat waves. It also serves as a proxy for vegetation water use, making it a critical tool for designing resilient green cities. Despite its importance, high-resolution mapping of urban ET that captures both spatial and temporal dynamics remains limited. This study focuses on the Paris metropolitan area, analyzing ET variability across multiple spatial scales (from 10 m to 10 km) using Sentinel-2 data from the Copernicus system. The Normalized Difference Vegetation Index (NDVI) is calculated with observation scale of 10 m, and then used as a proxy for ET. Universal Multifractal analysis, which have been widely used to characterize and model geophysical fields extremely variable across wide range of space-time scales, are implemented on this new data set. This framework is parsimonious since it basically relies on three parameters only: the mean intermittency codimension C1, the multifractality index a and the non-conservation parameter H.  Specifically, the multifractality index α (1.3–1.5) and the mean intermittency codimension C1 (~0.02) were derived to quantify the spatial and temporal heterogeneity of ET. The analysis, spanning 2019–2023, revealed noticeable temporal and spatial variability in ET. The study focuses on a square region of approximately 60 km × 60 km within the area around Paris. This region was further divided into multiple portions of size ranging from 2 to 10 km to assess potential variability over the studied areas. By incorporating both yearly and monthly data, the analysis captured seasonal trends as well as interannual variability, with higher variability observed during the summer months, driven by increased vegetation activity and water demand. Spatially, yearly data was analyzed and ET variability was most pronounced in densely populated areas, such as central Paris, where anthropogenic influences dominate. In contrast, forested areas and urban parks demonstrated significantly more stable ET patterns, underscoring the moderating effect of vegetation cover. These findings highlight the critical role of urban greening in mitigating extreme variability and stress on urban ecosystems.

How to cite: Zhu, S., Gires, A., Schertzer, D., Tchiguirinskaia, I., and Maksimovic, C.: Temporal and Spatial Dynamics of Urban Evapotranspiration in Paris: A Multiscale Perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16203, https://doi.org/10.5194/egusphere-egu25-16203, 2025.

EGU25-17156 | Posters virtual | VPS20

Leveraging EO for Security and Resilience 

Michela Corvino and the Michela Corvino

The ESA Directorate of Earth Observation Programmes has been actively leveraging satellite-based environmental information to address fragility contexts, focusing on areas such as environmental crimes, crimes against humanity, cross-border crimes, and onset of crises. Over the past decade, ESA has explored digital intelligence crime analysis by employing advanced data mining and machine learning tools to uncover hidden patterns and relationships in historical crime datasets, enabling better detection, prediction, and prevention of criminal activities.

Despite these advancements, the integration of Earth Observation (EO) capabilities into investigative practices remains limited. This is due to several challenges, including low awareness of EO's potential, a lack of illustrative use cases showcasing its benefits, inconsistencies in satellite data collection compared to investigative needs, high costs of very high-resolution imagery, and restricted access to national intelligence sources. To overcome these barriers, ESA has been investigating strategies to systematically incorporate EO-derived information into investigative frameworks also as legal evidence, aiming to enhance situational awareness and support stakeholders in developing procedures to exploit EO and OSINT for addressing international crimes and assessing fragility contexts, in cooperation with international organizations including Interpol, UNODC and ICC.

Recent developments in EO technology and methodologies have created significant opportunities for more impactful applications. ESA has focused on tailoring EO-based services and OSINT to meet the case-sensitive requirements of security and development end-users, enabling better integration of EO-derived insights into intelligence models. These efforts include developing advanced EO information products that go beyond routine offerings, testing and evaluating these products in collaboration with end-users, and demonstrating their value in operational settings.

The GDA Fragility, Conflict, and Security initiative has been a cornerstone of ESA’s work, involving partnerships with International Financial Institutions (IFIs) to co-design tools that provide precise and timely information. These tools have supported initiatives aimed at reducing inequalities, promoting economic development, and enhancing environmental safety in fragile and conflict or post conflict-affected areas. By combining geospatial data with diverse data sources, ESA has delivered customized analyses and reports to improve emerging threats analysis and decision-making processes.

Several ESA initiatives have demonstrated the benefits of EO services for assessing fragility risk exposure, characterizing dynamic needs in fragile contexts, planning post-conflict reconstruction, and managing natural resources. ESA constantly engages with stakeholders, including the OECD, security organizations, and humanitarian actors, and its community of industries and research centres to promote the adoption of EO in international development, humanitarian aid, and peacebuilding. Through these efforts, ESA continues to advance the role of EO in supporting justice, accountability, and sustainable recovery in fragile settings.

How to cite: Corvino, M. and the Michela Corvino: Leveraging EO for Security and Resilience, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17156, https://doi.org/10.5194/egusphere-egu25-17156, 2025.

EGU25-17965 | ECS | Posters virtual | VPS20

Lagrangian Evolution of the Trapping Capacity of Mesoscale Eddies in the Canary Eddy Corridor: A Numerical Modeling Approach 

Daniel Vacca, Borja Aguiar-González, and Tammy Morris

The Canary Eddy Corridor is a dynamic region of mesoscale eddy activity, playing a critical role in the transport of physical properties (heat and salt) and biogeochemical properties (nutrients, larvae, plankton) in the eastern North Atlantic. This study investigates the Lagrangian evolution of the trapping capacity of mesoscale eddies according to their lifecycle phases and vertical structure (surface vs. subsurface eddies).


We combine OceanParcels (an open-source Python toolbox) and an eddy identification and tracking algorithm with the GLORYS12V1 reanalysis product and altimetry data from AVISO to simulate particle release and track trajectories within eddies. Applying the eddy tracking algorithm at surface and subsurface levels in GLORYS12V1 reveals that subsurface eddies with a surface signal exhibit subsurface rotational velocities at the eddy core that occasionally exceed those of surface eddy cores. This highlights the potential misrepresentation of eddy transport capacity when relying solely on altimetry data, without accounting for the vertical structure, which can be better resolved through a combination of model outputs and observational data, such as non-standard Argo float configurations. Furthermore, a detailed analysis of the eddy lifecycle phases shows that mature eddies exhibit substantially greater trapping depths compared to their growth and decay stages. These findings align with earlier modeling analyses of dipoles originating south of Madagascar, which also highlight enhanced trapping depths in mature eddies.


The results provide a comprehensive view of the trapping capacity of mesoscale eddies throughout their lifecycle and vertical structure, emphasizing their critical role in biophysical coupling, ecological connectivity, and the transport of biogeochemical properties, as well as microplastics and other pollutants.

 

Acknowledgments: The first author is grateful for the internship grants ERASMUS +, AMI-MESRI, and TIGER. 

How to cite: Vacca, D., Aguiar-González, B., and Morris, T.: Lagrangian Evolution of the Trapping Capacity of Mesoscale Eddies in the Canary Eddy Corridor: A Numerical Modeling Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17965, https://doi.org/10.5194/egusphere-egu25-17965, 2025.

EGU25-18606 | ECS | Posters virtual | VPS20

Deep Learning based Paddy Land Abandonment Detection Using Multitemporal Polarimetric SAR Patterns 

Shivam Kasture, Aishwarya Hegde A, and Pruthviraj Umesh

The abandonment of agricultural land in India, especially paddy fields, has emerged as a significant challenge for food security and ecosystem sustainability in the country. Although rice production is vital for national food security, research on paddy land abandonment in India remains limited. Some Indian states have reported an alarming decline in paddy cultivation area over the past two decades. The study employs the Udupi district of Karnataka, India, a high-rainfall coastal region where paddy has traditionally been the dominant crop and where paddy land abandonment has been observed, as the study area. This study addresses crucial research gaps by framing these objectives for the study: (1) developing a deep learning framework that utilizes both intensity and phase information from polarimetric Synthetic Aperture Radar (SAR) data for abandoned paddy land detection, (2) leveraging recurrent neural networks (RNNs) to capture temporal patterns in abandonment, and (3) demonstrating an automated, all-weather monitoring approach that overcomes the limitations of traditional optical remote sensing in tropical regions.

Conventional monitoring approaches struggle with persistent cloud cover in tropical regions which limits effective assessment of abandonment patterns. SAR data provides unique capabilities for continuous monitoring under all weather conditions, making it particularly well-suited for tropical regions. However, previous studies have primarily underutilized SAR's potential by concentrating solely on backscattering intensity from ground range detected (GRD) products, overlooking the valuable phase information that could offer deeper insights into land use changes.  In this study, we employ Sentinel-1 Single Look Complex (SLC) data, which offers both intensity and phase information. Considering the temporal nature of paddy land abandonment, we developed a deep learning framework utilizing RNNs viz. LSTM, BiLSTM and BiGRU to effectively capture time-series patterns in the data. This framework analyzes backscattering coefficients (VV and VH polarizations) and polarimetric parameters (entropy, anisotropy and alpha angle) derived from SLC data collected during the Kharif seasons from 2017 to 2024. We carried out extensive ground truth data collection of active and abandoned paddy lands to train and validate our models. The backscattering coefficients were processed through orbit correction, radiometric calibration, TOPSAR deburst, multi-looking, speckle filtering and terrain correction. For deriving the polarimetric parameters, after basic preprocessing steps, the covariance matrix was generated followed by the polarimetric decomposition of the phase-preserved data. Results indicate that our RNN models show promising performance in detecting temporal patterns of paddy land abandonment. The method exhibits a robust ability to produce reliable abandoned land maps in regions prone to cloudy and rainy conditions. Future research should explore polarimetric features across various vegetation types in abandoned lands, expand the methodology to other agricultural systems, and examine the impact of socio-economic and topographical factors on abandonment patterns to support evidence-based land management policies.

How to cite: Kasture, S., Hegde A, A., and Umesh, P.: Deep Learning based Paddy Land Abandonment Detection Using Multitemporal Polarimetric SAR Patterns, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18606, https://doi.org/10.5194/egusphere-egu25-18606, 2025.

EGU25-19070 | Posters virtual | VPS20

Rainfall Dynamics in Wind Energy Scenarios 

Martin Obligado and Auguste Gires

The presence of rain in wind farms involves several modeling challenges, as the momentum exchanges between turbulent wakes and the particle phase present subtle phenomena. For instance, rain droplets are typically large enough to exhibit inertia relative to the air carrier phase. Under these conditions, it has been found that the gravitational settling of particles in turbulent flows may be either enhanced or hindered compared to stagnant conditions. While this has significant implications for rainfall transport, ash pollutants, and pollen dispersion, very few studies have been conducted in field conditions. Moreover, the scaling laws and non-dimensional parameters governing this phenomenon have not yet been properly identified, and determining which configurations result in the enhancement or hindrance of settling velocity remains an open question.

We propose a hybrid experimental/numerical approach. Field data from a meteorological mast located at a wind farm in Pays d’Othe, 110 km South-East of Paris, France, were used to characterize the background turbulent flow through a set of sonic anemometers. Additionally, disdrometers were employed to characterize the settling velocity of raindrops, discriminating by particle size. Numerical simulations complement this data analysis. Specifically, 3D space and time vector fields that realistically reproduce the observed spatial and temporal variability of wind fields are generated using multifractal tools. Then, 3D trajectories of non-spherical particles are simulated and their settling velocity derived.

Our findings indicate that the presence of turbulence significantly hinders the settling velocity of raindrops in turbulent environments. Our study covers several distinct rainfall events, allowing us to analyze the influence of turbulent flow properties on this phenomenon.

How to cite: Obligado, M. and Gires, A.: Rainfall Dynamics in Wind Energy Scenarios, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19070, https://doi.org/10.5194/egusphere-egu25-19070, 2025.

EGU25-19225 | Posters virtual | VPS20

Customizing Trends.Earth for land degradation assessment in the earth critical zone: a FAIR-EASE approach 

Italia Elisa Mauriello, Giuliano Langella, Fabio Terribile, and Marco Miralto

Land degradation is a critical challenge to sustainable development, impacting ecosystems, economies, and communities globally. As part of the FAIR-EASE Earth Critical Zone (ECZ) pilot, this study develops a tailored Land Degradation Assessment tool based on the Trends.Earth approach. The tool aims to enhance data accessibility, integration, and usability across environmental domains, supporting decision-making and policy frameworks aligned with the United Nations Sustainable Development Goals (SDGs).
Building upon the robust Trends.Earth implementation, we can integrate customized workflows and datasets to reflect regional variability in degradation indicators, including vegetation productivity, soil health, and land cover changes. Our approach prioritizes FAIR (Findable, Accessible, Interoperable, and Reusable) principles to ensure broad usability and collaboration across scientific and policy communities.
Preliminary results demonstrate the tool's capacity to enhace the detail of the analysis and to identify degradation hotspots. Furthermore, the integration of open-source geospatial tools and standards supports a scalable framework applicable to diverse environmental contexts.
The tool is designed to be embedded within the LandSupport platform, a geospatial decision support system, further enhancing its accessibility and integration into decision-making processes for land management.
This work contributes to advancing interdomain digital services and illustrates the potential of FAIR principles in addressing complex environmental challenges. We invite feedback from the community to refine, expand and customise the tool's application, fostering collaboration for sustainable land management.

How to cite: Mauriello, I. E., Langella, G., Terribile, F., and Miralto, M.: Customizing Trends.Earth for land degradation assessment in the earth critical zone: a FAIR-EASE approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19225, https://doi.org/10.5194/egusphere-egu25-19225, 2025.

EGU25-20653 * | Posters virtual | VPS20 | Highlight

The turbulence of solids: a multifractal plate tectonic model with Guttenberg-Richter plate “quakes”  

Shaun Lovejoy, Andrej Spiridonov, and Lauras Balakauskas

Over thirty years ago, Y. Kagan speculated that seismicity could fruitfully be considered as “the turbulence of solids”.  Indeed, fluid turbulence and seismicity have many common features: they are both highly nonlinear with huge numbers of degrees of freedom.  Beyond that, Kagan recognized that they are both riddled with scaling laws in space and in time as well as displaying power law extreme variability and – we could add – multifractal statistics.

Kagan was referring to seismicity as usually conceived, as a sudden rupture process  occurring over very short time periods.  We argue that even at one million year time scales, that the movement of tectonic plates is “quake-like” and is quantitatively close to seismicity, in spite of being caused by relatively smooth mantle convection. 

To demonstrate this, we develop a multifractal model grounded in convection theory and the analysis of the GPlates data-base of 1000 point trajectories over the last 200 Myrs.  We analyzed the statistics of the dynamically important vector velocity differences where Dr is the great circle distance between two points and Dt is the corresponding time lag.  The longitudinal and transverse velocity components were analysed separately.  The longitudinal scaling of the mean longitudinal difference follows the scaling law <Δv(Δr)> ≈ ΔrH with empirical H close to the mantle convection theory value  H = 1.  This high value implies that  mean fluctuations vary smoothly with distance.  Yet at the same time,  the intermittency exponent C1 is extremely high (C1 ≈ 0.55) implying that from time to time there are enormous “jumps” in velocity: “Plate quakes”.  For comparison, laminar (nonturbulent) flow has H = 1 but is not intermittent (C1 = 0), whereas fully developed isotropic fluid turbulence has the (less smooth) value H = 1/3 (Kolmolgorov) but with non-negligible intermittency C1 ≈ 0.07 and seismicity has very large C1 ≈ 1.3.  Our study thus quantitatively shows how smooth fluid-like behaviour for the longitudinal velocity component can co-exist with highly intermittent quake-like behaviour.

Whereas the longitudinal component is well modelled by (highly intermittent) convection, the transverse velocity is well modelled by Brownian motion.  In the temporal domain both components (including their strong correlations) display such diffusion behaviour (i.e. with classical exponent H = ½), but are highly intermittent (C1time = C1space/2 ≈ 0.27).  Finally, the extreme velocity differences (that appear as occasional spikes in the velocities) have power law probability tails; the “Guttenberg-Richter” exponents in the seismology literature.

The advection - diffusion model is based on an underlying multifractal space-time cascade process.  Using mantle convection theory, we show how the driving multifractal flux (ψ) is related to vertical heat fluxes, expansion coefficients, densities, viscosities and specific heats. Taking typical values predict driving fluxes very close to the observed mean <ψ> ≈ 1/(400 Myrs).  Trace moment analysis shows that the outer space-time scales of the cascade process are ≈17000 km in space and ≈ 50Myrs in time.   Whereas the former corresponds to half the Earth’s circumference, the latter is the typical time required for a plate to randomly “walk” the same distance.

How to cite: Lovejoy, S., Spiridonov, A., and Balakauskas, L.: The turbulence of solids: a multifractal plate tectonic model with Guttenberg-Richter plate “quakes” , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20653, https://doi.org/10.5194/egusphere-egu25-20653, 2025.

NP0 – ITS sessions

EGU25-503 | ECS | Posters on site | ITS1.3/NP0.2

Effects of Climate Change on Residential Energy Structure 

MengTing Zhu, Mengqi Zhao, Rongqi Zhu, Fengqiao Mei, and Yang Ou

Climate change may influence energy demand, with shifts in energy needs not only altering the energy structure but also posing challenges to the sustainability and resilience of energy systems. These impacts could further complicate the feasibility of achieving decarbonization goals. Residential energy sector is a critical component of global energy consumption. As temperature fluctuates and weather variability intensifies, households will adapt energy use to maintain comfortable living conditions. Energy consumption may increase due to climate change, but the magnitude remains uncertain. Considering various income groups around the world, residents may react to climate change heterogeneously.

Traditionally, some models use Heating Degree Days (HDD) and Cooling Degree Days (CDD) to serve as index of temperature change, which are often calculated by formulas below, where i means gridded cell, j means region,  means daily temperature, and represents comfortable temperature,  means population. First, calculate gridded HDD/CDDs as the difference between daily temperature and comfortable temperature. Then aggregate the gridded daily HDD/CDDs to region.

  (1)

   (2)

                                      (3)

However, calculation for HDD/CDDs still have several aspects that could be further improved. First, most temperature data used are predicted on SRES, and HDD/CDDs are assumed to be constant, so HDD/CDDs need to be updated to better reflect future climate change. Second, previous calculation always neglects the impact of crucial factors such as GDP when aggregating gridded temperature difference to regional level, only considering population distributional effects. Third, the difference resulted from income and climate also should be considered, for rich residents can afford more energy consumption, and long-term climate also impact response of people when faced with climate change.

Considering potential shortcomings mentioned above, we update the global HDD/CDDs of 32 regions in Global Change Analysis Model (GCAM). First, we use daily temperature data predicted by four climate models under different Shared Socioeconomic Pathways (SSPs) combining Representative Concentration Pathways (RCPs) scenarios from the Coupled Model Intercomparison Project Phase 6 (CMIP6), thus bridging the gap between climate model and GCAM. For in GCAM climate input module, HDD/CDDs are calculated based on historical climate data and are lack of fine-scale calculation. Second, our calculation adopts two weighting methods considering influence of population and GDP distribution on residential energy demand respectively. Third, beyond global-scale calculation, we refine calculation for China to the provincial level.

Fig. 1 Research Framework

Based on the updated HDD/CDDs, we use GCAM to analyze how climate change impact residential energy demand, aiming to provide scientific support for formulating policies that address the challenges posed by climate change to energy system. Our analysis offers comprehensive insights into residential energy demand change under SSPs and RCPs scenarios, accounting for income heterogeneity. These findings are informative to design effective mitigation policies in the context of climate change.

How to cite: Zhu, M., Zhao, M., Zhu, R., Mei, F., and Ou, Y.: Effects of Climate Change on Residential Energy Structure, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-503, https://doi.org/10.5194/egusphere-egu25-503, 2025.

Digital city contributes to improving resource allocation efficiency and quality of life, with a key component being the division of functional areas. This division directly influences the optimal allocation of urban spatial resources and the efficient operation of various services. However, a mismatch exists between virtual and physical city functions. For instance, many office activities do not occur in physical office spaces. In this study, Guangzhou is taken as the research area to quantify this mismatch in office spaces, utilizing mobile signaling data and POI (Point of Interest) data, and analyzing the factors influencing the mismatch. Mobile signaling data, combined with office software usage records, reveals the precise locations of office activities from a virtual perspective. POI data provides detailed records of physical office locations, while also encompassing other potential locations where office activities may take place. This study reveals the spatial characteristics and influencing factors of this mismatch in Guangzhou, provides scientific support for the development of digital cities.

How to cite: Jiang, H.: Quantifying spatial mismatch between virtual and physical office spaces, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1372, https://doi.org/10.5194/egusphere-egu25-1372, 2025.

EGU25-3332 | Orals | ITS1.3/NP0.2

Scaling Properties of Carbon Emissions in US Cities: Bigger is Better 

Kevin Gurney, Pawlok Dass, Jose Lobo, and Shade Shutters

The Vulcan Project version 4.0 emissions data product has generated all fossil fuel CO2 emissions across the US landscape, every hour, from 2010-2022 down to the scale of neighborhoods. From this complex landscape, we have extracted FFCO2 emissions for every urban area, following multiple commonly used urban definitions. The information extracted includes both Scope 1 and Scope 2 emissions with a wide array of “functional” attributes such as sector, fuel, vehicle class, building class, road class, and industrial sub-sector. Here, we analyze ~4000 US cities in terms of their size scaling properties. In particular, urban scaling properties provide novel insight into emergent properties such as the relationship between urban metabolism and urban size properties. This relationship varies by region and is indicative of the relationship between urban form and economies of scale including implications for infrastructural development and urban sprawl.

How to cite: Gurney, K., Dass, P., Lobo, J., and Shutters, S.: Scaling Properties of Carbon Emissions in US Cities: Bigger is Better, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3332, https://doi.org/10.5194/egusphere-egu25-3332, 2025.

EGU25-4066 | ECS | Posters on site | ITS1.3/NP0.2

Understanding and recognition of geo-scenes based on multimodal spatial semantics to monitor complex urban systems 

Hanqing Bao, Lanyue Zhou, and Lukas Lehnert

Urban geo-scenes (UGS) are an abstraction of the basic units of cities. Understanding and functional recognition of UGS is crucial to balancing and optimizing urban spatial layout, rationally allocating urban resources, and enhancing urban resilience and vitality. To construct UGS, urban geo-objects (UGO) e.g., derived from remote sensing must be combined with semantic information, which has seldom be done so far.  Consequently, this study designed a UGS recognition framework based on multimodal deep learning. First, we use very high-resolution satellite data to derive UGOs. Second, the self-built SE-DenseNet branch is used to mine deep physical visual features and social semantics from satellite image data and auxiliary data (POI, building footprints from UGOs). Finally, we build an urban fabric graph model to mine spatial semantics between UGOs.  In addition, a spatial semantic fusion module is introduced for the collaboration and interaction of multi-modal and multi-scale features. We evaluate the effectiveness of the proposed framework in the complex Beijing and Shenzhen regions of China. The overall accuracy is 91.35% and 90.24% respectively, which is higher than the state-of-the-art multimodal methods. In addition, our study also emphasizes the key role of spatial relationships and distribution patterns of UGO in UGS recognition, and the addition of POIs and building heights improves the recognition accuracy. The multimodal UGS recognition framework based on urban fabric can more effectively understand urban functions, thereby achieving urban planning and management.

How to cite: Bao, H., Zhou, L., and Lehnert, L.: Understanding and recognition of geo-scenes based on multimodal spatial semantics to monitor complex urban systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4066, https://doi.org/10.5194/egusphere-egu25-4066, 2025.

EGU25-4759 | ECS | Orals | ITS1.3/NP0.2

Hybrid Intelligence and Explainable AI for Urban Growth Prediction Modelling 

Danish Khan and Nizamuddin Khan

The fast-evolving nature of urbanization and its complex patterns require precise and interpretable machine learning models to effectively predict urban growth. To address this challenge, this study introduces a novel framework combining Hybrid Intelligence and Explainable AI (XAI), specifically Shapley Additive Explanations (SHAP) to improve model performance, robustness, and transparency. Using a weighted ensemble technique, the proposed method systemically integrates linear, tree-based, and neural network models to propose a hybrid of Elastic Net, XGBoost, and Wide & Deep Neural Network (EN-XGB-WDN) frameworks for urban growth prediction. The methodology follows a multistep approach and includes the development of the hybrid model, its evaluation for binary classification, integration of SHAP-based feature analysis to identify key drivers of urban growth and improve model interpretability, retraining of the hybrid model to increase accuracy and reduce overfitting, and validation of the proposed framework using standard evaluation metrics including accuracy, precision, recall, F1 score, and AUC. The hybrid model achieves an overall accuracy of 87.34%, a weighted F1-score of 87.18%, and an AUC of 0.9442. The SHAP analysis revealed that Drive Time (DT), Distance from Roads (DfR), and Elevation are the most impactful features to understand the dynamics of urban growth. The findings revealed how variations in specific features, such as higher DT and lower DfR, significantly affect urban growth probabilities. The hybrid model also categorized urban growth probabilities into five classes: very low (40.62%), low (23.27%), moderate (15.38%), high (12.10%), and very high (8.63%), revealing spatial patterns of urban expansion. The framework combines hybrid ensemble methods with SHAP-based explanations to significantly enhance the predictive and explanatory power of urban growth models compared to the limitations of traditional approaches. This study highlights the efficiency of integrating hybrid machine learning and Explainable AI to understand and predict complex urbanization dynamics. The outcomes offer actionable insights for policymakers and urban planners, facilitating data-driven strategies for sustainable urban development. This research demonstrates the effectiveness of hybrid intelligence coupled with Explainable AI, offering a scalable and interpretable framework to better understand and predict urbanization patterns.

How to cite: Khan, D. and Khan, N.: Hybrid Intelligence and Explainable AI for Urban Growth Prediction Modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4759, https://doi.org/10.5194/egusphere-egu25-4759, 2025.

Urban geometry plays a key role in determining the urban climate through its complex shading and trapping effects on solar radiation. As a result, urban albedo is typically lower than rural albedo, suggesting a larger solar heat gain in urban areas. As cities grow larger and more heterogeneous in geometry, quantifying the impact of this variation on albedo at the city scale requires computationally efficient models that can also resolve the 3D geometry of real cities. To this end, we developed a simplified 3D urban radiation model and used it to examine the variations in albedo due to heterogeneous geometry in the city of Shanghai. The model reduces computational complexity from O(n²) to O(n) while maintaining an accuracy within 5% compared to traditional 3D models. The case study in Shanghai shows that albedo has a linear relationship with building height but varies nonlinearly with changes in building density. The lowest albedo occurs when the building density (λp) is around 0.2 and the building height-to-length (H/L) ratio is 6, while occurs at λp > 0.3 with H/L = 1. This suggests that optimizing building geometry could improve the urban climate and potentially being used to increase the utilization of solar energy.

How to cite: Zhou, H. and Wang, K.: Development of simplified 3D urban radiation model to examine the variations of albedo due to heterogenous geometry in the city of Shanghai, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4805, https://doi.org/10.5194/egusphere-egu25-4805, 2025.

EGU25-5462 | Orals | ITS1.3/NP0.2

Remote sensing-driven analysis of hourly urban heat storage and its effects on urban heat islands in China 

Nana Li, Fengxiang Guo, Junxia Dou, Yanfei Ma, and Shiguang Miao

Urban heat storage (Qs) is an essential component of urban surface energy balance. Urban with 3D structure has larger surface area than rural and urban would absorb and release more energy than rural. Qs is the main factor for urban heat island (UHI) at nighttime. The quantitative contribution of Qs to UHI is still unclear, due to the lack of a spatio-temporal continuous Qs dataset. In this study, firstly, we developed an urban surface thermal inertia model considering diurnal variation of surface temperature (LST) using hourly LST of Himawari-8. Secondly, the hourly Qs at 2-km resolution in three urban agglomerations in China was simulated by a half-order time derivative method which derived from combining the one-dimensional heat diffusion equation and Fourier’s law for heat conduction, using the urban thermal inertia model and hourly Himawari-8 LST. Thirdly, the relationship between Qs and air temperature (Ta) was studied at different time scales (day and nighttime, four seasons) and different LCZs (local climate zones). The Ta was derived from the interpolation of dense automatic weather stations with more than 10000 sites in China. Finally, some urban heat mitigation measures were provided based on the above analysis. Based on the in-situ observation, the accuracy of urban thermal inertial in this study was higher than other model, RMSE, MAE, R2 were improved from 4.65 K, 3.58 K and 0.88 to 1.86 K, 1.53 K and 0.97. In addition, the simulated Qs were validated by the observed Qs (the minus of net radiation, sensible and latent heat flux from in-situ flux tower, and anthropogenic heat flux simulation) in Beijing, Shanghai and Guangzhou, R2 could be up to 0.92. The results showed that, Qs was more consistent with Ta at nighttime than daytime, with R2 of 0.96 and 0.1, respectively. That showed that Qs is the main factor for nighttime UHI in this study area. During nighttime, the high-rise building has higher Ta than low-rise building, due to higher Qs and release more energy than low-rise. In natural surfaces, water has larger Qs and higher Ta than dense trees. The loop (between hourly Qs and hourly Ta) shape were different at different LCZs, with different loop area and loop slope. Based on the loop area and slope, we found that high-rise building had higher UHI but varied quickly, however, low-rise UHI is lower but would last longer. The water surface in nighttime is also heat source and has a longer time UHI. Therefore, the high-rise building and water surface are not conductive to alleviating the nighttime UHI.

How to cite: Li, N., Guo, F., Dou, J., Ma, Y., and Miao, S.: Remote sensing-driven analysis of hourly urban heat storage and its effects on urban heat islands in China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5462, https://doi.org/10.5194/egusphere-egu25-5462, 2025.

EGU25-6392 | ECS | Posters on site | ITS1.3/NP0.2

Do people-oriented urbanization catch up with land and population urbanization in China? 

Tianci Gu, Qingxu Huang, and Yiming Hou

China has undergone rapid urbanization in terms of population and land use in recent years. However, there are notable lags in "people-oriented" dimensions of urbanization, including urban social services, environmental sustainability, and equity. Here, considering the complex interactions of sub-components of urbanizations, we examined 16 "people-oriented" urbanization indicators across four dimensions - economic, social, environmental, and equity dimensions - from 2005 to 2020. Using methods such as paired t-tests and the evenness measurement, we analyzed and identified the dynamic relationships between these 16 indicators with population/land urbanization at multiple scales, including national, regional, urban agglomeration, and different city sizes. We found that between 2005 and 2020, China's urbanization indicators showed an overall upward trend, with changes ranging from 1.09 to 53.95 times. Among "people-oriented" urbanization indicators, economic and social indicators lagged behind land and population urbanization, while environmental indicators took the lead. The evenness index among indicators showed a "U-shaped" change pattern. Particularly since the implementation of China's New-type Urbanization Plan in 2014, the evenness index among indicators gradually increased from 35.43 to 37.39 in 2020, representing a 6.9% improvement. Looking forward, it is necessary to strengthen investment in social service systems and implement placed-based coordination strategies to promote further development and balanced growth of "people-oriented" urbanization.

How to cite: Gu, T., Huang, Q., and Hou, Y.: Do people-oriented urbanization catch up with land and population urbanization in China?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6392, https://doi.org/10.5194/egusphere-egu25-6392, 2025.

EGU25-6870 | Posters on site | ITS1.3/NP0.2

Exploring Switzerland's Rural-Urban Continuum Through Unsupervised Learning 

Marj Tonini, Jingyan Yu, and Alex Hagen-Zanker

In recent decades, urban expansion across Europe has accelerated, driving the rapid growth of rural-urban interfaces. The increasingly complex and dynamic nature of territorial transitions calls for the timely development of classification systems designed to systematically organize areas along a spectrum, from distinctly urban to distinctly rural. Current classifications often rely on predefined criteria, such as population size and density, which may not fully capture the nuanced and evolving nature of transitions driven by the complex interplay of socioeconomic processes, demographic shifts, environmental factors, and dynamic geographic forces.

This research addresses existing gaps by employing modern data-driven approaches, including machine learning and clustering techniques, to develop adaptive typologies that integrate diverse demographic, socioeconomic, and environmental variables. Using Switzerland as a case study, the proposed methodology offers a dynamic and scalable framework for territorial classification, supporting the effective management of territorial transitions and landscape conservation in Alpine regions. The analysis leverages a multidimensional dataset derived from the 2020 official census, incorporating 18 variables that encompass demographic profiles, socio-economic, and the physical space characteristics.

We used Self-Organizing Map (SOM) combined with hierarchical clustering. SOM, a type of competitive learning neural network, reduces the complexity of high-dimensional data by mapping it onto a two-dimensional grid of neurons. Visual outputs, such as heatmaps, enhance the interpretation of trends and patterns, providing a clearer understanding of variables distributions and interrelationships. Afterward, the SOM output grid of neurons was aggregated into six distinct clusters, which were mapped onto the geographical space. This produced a visual representation of the spatial organization of territorial typologies along the rural-urban continuum in Switzerland at a detailed municipal level.

The data-driven clustering approach developed in this study proved effective in capturing the complex and diverse nature of Swiss territorial typologies. The key findings reveal a landscape marked by a complex rural-urban interface, extensive intermediate zones, and significant spatial fragmentation. These final six territorial typologies could be characterized as follows: urban centres, representing the main hubs at the highest level of the Swiss urban hierarchy; suburban areas, located near and well-connected to urban centres; two peri-urban areas, distinguished into aging-rural areas and rural-urban edge; rural-forest areas, situated at medium to high elevations, featuring a forested landscape and rural settings; unproductive areas, encompassing high-altitude regions and including critical Alpine glaciers.

How to cite: Tonini, M., Yu, J., and Hagen-Zanker, A.: Exploring Switzerland's Rural-Urban Continuum Through Unsupervised Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6870, https://doi.org/10.5194/egusphere-egu25-6870, 2025.

Adequate sunlight exposure is crucial for human wellbeing, yet its accessibility in cities is significantly compromised by both could cover and complex three-dimensional (3D) urban structure. Here we adopted an analytical framework that integrated natural day length variations, cloud cover effects, and 3D urban structure to quantify actual sunlight duration in urban areas. By using high-resolution satellite products, fine-scale canopy height data, and detailed 3D building footprints, we mapped the spatiotemporal patterns of sunlight availability and quantified the relative contributions of cloud cover and urban structures on the loss of sunlight for Chinese cities. Our analysis reveals pronounced spatial disparities and trends in urban sunlight resources in China, underscoring the urgent need for evidence-based urban planning strategies that optimize natural light accessibility for sustainable urban development.

How to cite: Wu, X. and Chen, B.: Quantifying urban sunlight accessibility across Chinese cities: Impacts from cloud cover and three-dimensional (3D) urban structure, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7638, https://doi.org/10.5194/egusphere-egu25-7638, 2025.

EGU25-7834 | ECS | Posters on site | ITS1.3/NP0.2

Advancing Urban Environment Studies in Murcia, Spain through an Automated Façade Image Classification Model 

Maria Isabel De La Cruz Luis, Sandra Martinez Cuevas, César Garcia Aranda, Maria del Carmen Morillo Balsera, and Enrique-Maria Poveda Lorente

Over the past few decades, the rapid growth of cities has evolved into a significant social, demographic, and architectural phenomenon, highlighting the vital importance of urban planning in fostering sustainable development. In this context, machine learning has emerged as a game-changing discipline, utilizing advanced algorithms to reshape traditional approaches to urban data management and analysis.This study combines Geographic Information Systems (GIS), Deep Learning techniques, and verified data from the General Directorate of the Spanish Cadastre to perform a comprehensive analysis of the urban environment through façade images in Murcia, one of Spain’s most dynamic metropolitan areas.Leveraging the clustering analysis of the studied variables, an automated binary classification model for façade images was developed using the pretrained EfficientNetB0 architecture in Python. To enhance interpretability, heat maps were generated to visualize the regions the model focuses on during classification. These heat maps reveal the critical features of the facades that guide the model’s decisions, providing valuable insights into the key factor influencing the classification process.The results were integrated into ArcGIS PRO, using the cadastral reference of the properties as a key attribute for a detailed spatial analysis. This approach revealed two significant areas linked to the metropolitan growth of Murcia, laying a strong foundation for future urban studies in the region.

Funding: Twin-ER: Earthquake Risk Pilot Digital Twin. Grant PID2023-149468NB-I00, funded by MCIU/AEI/10.13039/501100011033 and FEDER/EU

How to cite: De La Cruz Luis, M. I., Martinez Cuevas, S., Garcia Aranda, C., Morillo Balsera, M. C., and Poveda Lorente, E.-M.: Advancing Urban Environment Studies in Murcia, Spain through an Automated Façade Image Classification Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7834, https://doi.org/10.5194/egusphere-egu25-7834, 2025.

EGU25-8416 | Posters on site | ITS1.3/NP0.2

Measuring global human access to essential daily necessities and services 

Bin Chen, Shengbiao Wu, Andy Nelson, and Peng Gong

Equitable access to daily necessities and services is crucial for enhancing human quality of life and is integral to achieving the United Nations’ Sustainable Development Goals. However, knowledge about global access to these essential resources remains limited and fragmented, primarily due to the absence of a comprehensive infrastructure inventory and scalable measures of accessibility. Here we compiled the most extensive global database of points of interest (POI) to represent six essential infrastructure categories—living, healthcare, education, entertainment, public transit, and work. We used refined 30-meter resolution friction surface data to map travel times to these critical infrastructures as a proxy for accessibility across the urban-rural continuum and assessed disparities across geographic, urbanization, and socio-economic contexts. Our results reveal that access to daily necessities and services is unevenly distributed in terms of total infrastructure, per capita availability, and travel time. Globally, only 38.7% (2.6 billion people) and 50.7 % (3.4 billion people) of the population resides within a 15-minute and 30-minute walking distance of essential daily necessities and services, respectively. These results highlight the urgent need to optimize strategies for planning, allocation, and management of critical infrastructure to promote inclusive and sustainable development.

How to cite: Chen, B., Wu, S., Nelson, A., and Gong, P.: Measuring global human access to essential daily necessities and services, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8416, https://doi.org/10.5194/egusphere-egu25-8416, 2025.

Evaluating human interaction with environmental health determinants in space and time is fundamental to estimate personal environmental exposures. The increasing demand in an exposure assessment of entire populations requires to combine environmental variables at high resolution on large spatial extent, e.g. at nationwide or continental scale, with the space-time activity pattern of each individual in a study population.

Modelling population health and citizens' exposures is a complex process involving multiple procedural steps. One major step is to generate spatio-temporal information on environmental factors, either considered as beneficial for human wellbeing, for example, accessibility to green space or blue space, or considered as having negative health impacts such as the existence of air pollution, noise or heat. To capture the spatial variability these datasets need to be generated at high resolution. To allow for studies comparing cities, regions or countries, a geographical extent of subnational or larger size is required. In addition, data can be temporal to cover diurnal or seasonal variation of an environmental variable. Another major step is to use the environmental factors to as input to models calculating exposures for entire study populations, ranging from a few hundred participants up to millions of citizen. Here, socio-economic variables, mobility, different travel modes, and other daily activities with accompanying location changes need to be considered to mimic the space-time paths of each participant of a study population. These tasks require sufficient flexibility in both constructing environmental models as well as executing those eventually on HPC systems to break computational barriers of common workstations.

We present a computational framework for implementing both procedural steps and show the development of two European scale raster maps on a 25m grid and their subsequent usage to estimate human exposures to greenness visibility and noise. The maps were created with LUE (https://lue.computationalgeography.org/), an open-source modelling framework providing a Python package with currently 115 general-purpose operations for the construction of spatio-temporal simulation models. We implemented two custom focal operations that make use of the LUE framework. The first focal operation calculates for each raster cell the visible green area within a particular buffer size (c.f. Labib 2021, https://doi.org/10.1016/j.scitotenv.2020.143050). The second focal operation aggregates traffic-related noise within a particular buffer size, considering attenuation due to geometric divergence, atmospheric absorption, ground effects and diffraction.

We calculated visible green within a radius of 800m and noise within 1500m radius using 768 CPUs on eight HPC cluster nodes, and then used Campo (https://campo.computationalgeography.org/) for activity-based exposure assessment. The obtained exposure estimates can show considerable differences for different typical human activity patterns, such as homemaker or commuter, as well as a high spatial variability.

How to cite: Schmitz, O., de Jong, K., Shen, Y., and Karssenberg, D.: Assessing human exposures to environmental risk factors at continental-scale: accounting for short range variation in environmental factors and human activity patterns, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8801, https://doi.org/10.5194/egusphere-egu25-8801, 2025.

Anthropogenic heat generated by building energy use contributes to the urban island and climate change. Quantifying high spatiotemporal resolution city scale building energy use (BEU) and anthropogenic heat emission (AHE) is necessary for understanding urban microclimate and sustainable development. However, the current shortage of such data is insufficient to support urban energy management and climate decision-making. We estimated BEU and AHE from buildings in Hong Kong using a GIS-based city-scale building energy model (GIS-CBEM) and investigated their spatiotemporal variations. First, all buildings were categorized into 11 types, and a prototype was developed for each type. These prototypes were then calibrated using annual building energy consumption data from surveys. We studied the energy use profile for each building prototypes under the Typical Meteorological Year (TMY) weather data. Then, we estimated hourly BEU and AHE for all buildings in Hong Kong at the individual building level. The study results unveiled the spatiotemporal variation of buildings in Hong Kong at high resolution and detected divergent structure of building end-use and fuel use for different building prototypes. We found that the total BEU of all buildings in Hong Kong peaked at 5.1 × 109 kWh in August, with 36.7% from HAVC system, while the lowest BEU was found in February at 3.5 ×109kWh, with 14.1% from HAVC system. Total AHE from all buildings reached a maximum of 8.1 × 109 kWh in July and minimum of 4.1 × 109 kWh in February. Our findings have critical significance in enhancing energy efficiency, reducing environmental impact, and promoting sustainable development.

How to cite: Liu, Q. and Zhou, Y.: Unveiling Spatial and Temporal Variations of Building Energy Use and Anthropogenic Heat Emissions in Hong Kong, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9314, https://doi.org/10.5194/egusphere-egu25-9314, 2025.

Traffic congestion continues to challenge urban development, yet most research emphasizes large-scale factors such as road layouts and land use, overlooking localized visual aspects encountered by drivers. This study employs geographically weighted random forest, a non-linear and spatially explicit method, to explore how localized visual features—such as vehicle density, building structures, greenery, and road conditions—impact traffic congestion in Chicago. By integrating transport network dynamics with visual streetscape characteristics, the geographically weighted random forest approach captures spatial heterogeneity and complex interactions more effectively than traditional models. Results demonstrate that incorporating these multi-scale features improves model fit, revealing that greenery mitigates congestion, while dense urban structures and vehicle clusters exacerbate delays. These results highlight the potential of integrating visual characteristics of streetscapes into urban strategies to address congestion more effectively.

How to cite: Xu, M. and Weng, Q.: Modeling the Spatial Dynamics of Traffic Congestion Through Street-Level Visual Features: Evidence from Street View Images in Chicago, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9394, https://doi.org/10.5194/egusphere-egu25-9394, 2025.

Exploring the effect of building morphology on Land Surface Temperature (LST) has received surging attention. In this process, a fundamental precondition is selecting an appropriate spatial statistical unit to calculate building morphological indices and corresponding LST. However, different units lead to divergent results, indicating they inevitably suffer from the Modifiable Areal Unit Problem (MAUP), which brings large uncertainties. This study places special emphasis on proposing a new spatial unit, the Homogenous Unit of Building Morphology (HUBM), to re-describe building morphology and re-analyze its effect on LST with less uncertainty. Results show: (1) building morphology portrayed by HUBM maintains more spatial characteristics and remains relatively stable across scales, which is more consistent with the realistic building environment. (2) The relationship identified by HUBM shows building morphology is not strongly correlated with LST in essence and is regarded as more authentic due to the more objective portrayal of building morphology, while this relationship may be overestimated by previous common units. (3) The effect of building morphology on LST explored by HUBM also remains relatively stable across different scales (R2 fluctuation amplitude of 0.08, 0.12, and 0.08 in the spring, summer, and winter, respectively) compared to regular grids (R2 fluctuation amplitude of 0.18, 0.2, and 0.2), effectively alleviating the uncertainty associated with the MAUP. These findings provide new insights into re-examining the authentic effect of building morphology on LST, assisting in addressing urban heat island effects and promoting sustainable urban development. Moreover, HUBM can be applicable to other urban issues for mitigating MAUP.

How to cite: Yang, L., Yang, X., and Li, S.:  Is 3D building morphology really related to land surface temperature? Insights from a new homogeneous unit, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10149, https://doi.org/10.5194/egusphere-egu25-10149, 2025.

EGU25-11618 | ECS | Orals | ITS1.3/NP0.2

Measuring resilience of urban areas using public data and a reproducible approach 

Ekaterina Tarasova and Massimiliano Alvioli

With rapid urbanization, cities face critical sustainability challenges, including poverty, resource shortages, pollution, and climate impacts. The EU Cities Mission supports 112 cities in developing Climate City Contracts to achieve climate neutrality by 2030 [1], emphasizing strategic, cross-sectoral approaches and stakeholder collaboration. This study introduces a systematic and indicator-based assessment of urban resilience, utilizing EU-sourced environmental, OpenStreetMap, and a few nationally sourced data. The methodology incorporates 12 key indicators, mapped at high resolution for 83 Italian cities using open-source GIS software [3], ensuring full reproducibility and applicability to other European cities. The indicators are categorized into five classes:

(i) nature and biodiversity, including forest canopy coverage, native habitat areas, biodiversity, geodiversity [4], ecological corridors, and heat island effects [5];

(ii) natural hazards, including susceptibility to flooding, earthquakes, wildfires, and landslides [6];

(iii) air pollution, including concentration of PM2.5 and NO2;

(iv) transport, including availability of sustainable and affordable transport systems;

(v) social indicators, including population living in close proximity to green spaces or water sources, and public services.

This study evaluates the current state of Italian cities [7], identifies regional differences, and highlights the strengths and weaknesses of each city individually, based on results provided by the urban indicators.

The software developed for this study is flexible, as the input data exists for the whole of Europe and it is easily extensible with modular scripts, to include additional indicators. The scripts processes data to produce spatially distributed results (raster maps) for each indicator in each class listed above and then summarize each indicator with a numerical figure.

Preliminary findings suggest significant regional variation in factors contributing to climate resilience and citizen well-being [8]. Cities in Northern Italy exhibit larger green space coverage but also higher air pollution levels. In contrast, Central Italy stands out for its high species biodiversity and geodiversity. Moreover, results uncover regional spatial patterns, offering actionable insights for policymakers to design locally informed and effective strategies. The findings contribute to advancing sustainability goals, supporting urban transformations toward enhanced resilience and reduced environmental impact. A comprehensive set of urban indicators, including those derived in this study and summarized into a single numerical output for each category, allows ranking of cities and promoting the adoption of data-driven strategies for sustainable development.

 

References

[1] United Nations (2023) https://sdgs.un.org/goals/goal11

[2] Sarretta et al., Int. Arch. Ph. Rem. Sens. Spat. Inf. Sci. (2021) https://doi.org/10.5194/isprs-archives-XLVI-4-W2-2021-159-2021.

[3] Neteler et al., Env. Mod. Softw. 31 (2012) https://doi.org/10.1016/j.envsoft.2011.11.014

[4] Burnelli et al., Geomorphology 471 (2024) https://doi.org/10.1016/j.geomorph.2024.109532

[5] Morabito et al., Sci. Tot. Env. (2021) https://doi.org/10.1016/j.scitotenv.2020.142334

[6] Loche et al., Earth-Science Reviews 232 (2022) https://doi.org/10.1016/j.earscirev.2022.104125

[7] Alvioli, Land. Urb. Plan. 204 (2020) https://doi.org/10.1016/j.landurbplan.2020.103906

[8] Boeing et al., Lancet Global Health 10 (2022) https://doi.org/10.1016/S2214-109X(22)00072-9

How to cite: Tarasova, E. and Alvioli, M.: Measuring resilience of urban areas using public data and a reproducible approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11618, https://doi.org/10.5194/egusphere-egu25-11618, 2025.

EGU25-13131 | Posters on site | ITS1.3/NP0.2

  Large Temperatures in Water Distribution Pipes as a Water Quality Threat: Measurements and Modelling 

Claus Haslauer, Ilja Kroeker, Elisabeth Nißler, Sergey Oladyshkin, Wolfgang Nowak, Holger Class, and Esad Osmancevic

Due to climate change, new challenges arise in drinking water infrastructure planning and in the re-assessment of well-established urban drinking water utilities. We observed temperatures exceeding 25 °C in drinking water supply pipes, which pose a health threat and water quality problem, as these temperatures are favorable for microbial growth.

We set out to predict temperatures in drinking water supply networks. The key step to achieve this goal is to monitor and model soil temperatures and soil moisture derived from meteorological forcing functions. With meteorological observations and soil material properties, we describe the heat transport and water flow from the ground surface into the subsurface and from there into the pipes and with the water in the pipes.

In order to achieve this goal, we solved the heat and water balances jointly at the atmosphere-subsurface interface, using the open-source numerical simulation framework DuMuX. We were able to do this because of the available meteorological observations (e.g., radiation balance, precipitation intensity) next to the newly installed pipes. These balances provide a novel interface condition for heat transport and water flow modelling. We coupled the heat transport through the drinking water pipe walls to the drinking water in the pipes and to the subsurface transport processes.

At a pilot site, we installed typical drinking water pipes (PE and cast iron), backfilled with known material (typical gravelly conditions below roads and naturally existing sandy clay), and applied land-cover (asphalt and natural vegetation). We were able to reproduce the joint measurements of temperatures and soil moisture under various conditions (well-draining gravel vs. less-draining clayey material; vegetation vs. asphalt).

In this presentation, we demonstrate results of the multi-year measurement campaign, the results of 1D and 2D subsurface heat transport models coupled to dynamic hydraulic conditions in the drinking water pipes, and an innovative surrogate-based Bayesian active learning-assisted model calibration methodology.

This work presents an important first step towards predicting temperatures in drinking water supply pipes and will be directly relevant for chemical and biological processes that occur in non-isothermal conditions (e.g., due to climate change), for example, in relation to contaminant remediation. Our results are of relevance for drinking water supply companies, shallow geothermal design, and urban planning.

How to cite: Haslauer, C., Kroeker, I., Nißler, E., Oladyshkin, S., Nowak, W., Class, H., and Osmancevic, E.:   Large Temperatures in Water Distribution Pipes as a Water Quality Threat: Measurements and Modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13131, https://doi.org/10.5194/egusphere-egu25-13131, 2025.

Urban climate modelling tools like the Surface Urban Energy and Water balance Scheme (SUEWS) are indispensable for investigating complex surface–atmosphere interactions and guiding urban adaptation strategies. However, these models often present substantial barriers to use: they require extensive technical know-how, involve intricate input datasets, and can be time-consuming to set up and interpret. Recent advancements in Large Language Models (LLMs) hold promise for bridging this gap by transforming complex domain-specific tasks—such as data validation, simulation setup, and error diagnosis—into user-friendly interactive experiences.

In this study, we propose a novel workflow that leverages LLM capabilities—such as generative text, code suggestion, and context-driven troubleshooting—to streamline SUEWS usage and improve accessibility for researchers and practitioners:

  • Automated Model Configuration
    We explore the use of LLM-guided prompts to generate properly formatted SUEWS input files, such as specifying hourly meteorological forcing data (e.g., temperature, wind speed, and humidity) or land cover fractions required for accurate simulations. By conversing with the model about location, time range, and data availability, users can rapidly produce consistent and error-checked setup files, reducing manual edits that often lead to inconsistencies.

  • Interactive Error Diagnosis
    LLMs can parse error logs and suggest potential solutions in real time. For example, if SUEWS outputs an error related to missing albedo values for a specific land cover type, the LLM can pinpoint the source of the issue and suggest default values or a method for calculation based on site-specific conditions. For example, if a runtime error indicates a mismatch in the date format of meteorological input data, the LLM can identify the exact line causing the error, recommend the correct format, and provide a command or script snippet to rectify the issue. Through iterative dialogue, the model clarifies the root causes of typical setup or runtime issues, explaining how to fix them without requiring the user to trawl through detailed documentation.

  • Model Output Interpretation
    Interpreting large volumes of SUEWS output, such as energy balance components (net radiation, latent heat flux, and sensible heat flux) or water budget terms (runoff and evapotranspiration), can be daunting, especially for newcomers. LLMs can summarise key metrics—like energy flux partitioning and surface runoff patterns—and highlight discrepancies in data, thereby assisting in rapid analysis and scenario comparison.

Our findings indicate that an LLM-enabled approach substantially lowers the learning curve and operational overhead associated with SUEWS, while still maintaining scientific rigour. We piloted trial deployments in teaching and professional contexts, reporting improvements in both setup speed and user confidence. Future work includes refining the LLM’s domain-specific training to ensure physically consistent responses—such as maintaining energy balance across flux computations or ensuring water budget closure—and incorporating advanced visualisation plugins for immediate data interpretation.

By harnessing the dialogic strengths of LLMs, we aim to remove barriers to the complexity of urban climate modelling, ultimately broadening participation and fostering more informed decision-making in cities worldwide.

How to cite: Sun, T.: Remove Barriers to Accessible Urban Climate Modelling with Large Language Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13462, https://doi.org/10.5194/egusphere-egu25-13462, 2025.

EGU25-13711 | ECS | Orals | ITS1.3/NP0.2

Compound heat and ozone pollution in urban areas 

Chenghao Wang, Xiao-Ming Hu, and Jessica Leffel

The frequent occurrences of heat wave events and air pollution episodes have become pressing global concerns. Concurrent heat and ozone pollution events, in particular, have been widely documented across various regions and often result in more severe impacts compared to isolated stressors, leading to increased mortality and morbidity rates. However, our understanding of these compound events in urban environments, particularly their dynamics under different background climates and urban settings, remains limited. In this study, we systematically characterized the frequency, intensity, and duration of compound heat and ozone pollution events during warm seasons across all urban areas in the continental U.S. using long-term, high-resolution daily air pollution and air temperature datasets. Results suggest that urban heat waves, defined by daily maximum temperature, were more frequent, more intense, and longer lasting than their rural counterparts, primarily due to the urban heat island effect. In contrast, over half of the U.S. cities experienced fewer, less intense, and shorter ozone pollution episodes than surrounding rural environments. The spatially heterogeneous disparities in ozone pollution episodes among cities are mainly attributed to whether ozone production is limited by VOC or NOx, as revealed by time series analyses. Despite the overall decreasing trend of surface ozone concentrations during the last two decades, 89% of U.S. cities experienced more frequent compound heat and ozone pollution episodes than rural areas. Additionally, the cumulative heat and ozone intensities were higher in 91% and 88% of U.S. cities, respectively, than in their rural backgrounds. The duration of compound events tends to be shorter in urban areas. These findings highlight the dependence of such compound events on local and background conditions, emphasizing the need for locally tailored mitigation plans to reduce their impacts. This study also calls for detailed regional numerical simulations to elucidate the mechanisms driving these events.

How to cite: Wang, C., Hu, X.-M., and Leffel, J.: Compound heat and ozone pollution in urban areas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13711, https://doi.org/10.5194/egusphere-egu25-13711, 2025.

EGU25-13868 | Orals | ITS1.3/NP0.2

Knowledge Networks help address urban flooding and water-energy challenges  

Lilit Yeghiazarian and the Knowledge Networks Team

Cities are highly interconnected networks of networks (referred to as the Urban Multiplex) that include the power grid and transportation networks, surface water and groundwater, sewerage and drinking water systems, inland navigation and dams – all intertwined with the natural environment and socioeconomic and public health sectors. While the Urban Multiplex is physically and functionally connected, the data produced within its individual sectors are not. This prevents us from fully understanding how the Urban Multiplex is connected, and how failures triggered by external stressors like floods cascade.  

Knowledge Networks are an AI technology that (i) integrates Urban Multiplex data, (ii) produces real-time flood forecasts across the continental U.S., (iii) serves as the foundation to evaluate the total impact of floods on cities, and (iv) supports queries at the nexus of water and energy. This talk will describe the development of the Urban Flooding and Water-Energy Nexus Open Knowledge Networks that aim to provide actionable answers to questions such as:

  • Real-time flood mitigation and response: Will my neighborhood flood? Will I have access to water and power? Will this storm disrupt the power grid, drinking water treatment plant, or a bridge?

 

  • Long-term design, planning and research: What is the total socioeconomic impact of this flood? Which critical urban infrastructure will likely fail in a future flood? Which failures will affect the most people or the most vulnerable people? Are there vulnerable communities downstream of this coal mine?

The interdisciplinary team behind this project has brought together academic researchers, industry, federal government, U.S. National labs and local stakeholders. It is funded by the U.S. National Science Foundation’s Convergence Accelerator Program that is structured to enable rapid advancement in highly complex problems of critical societal importance.

How to cite: Yeghiazarian, L. and the Knowledge Networks Team: Knowledge Networks help address urban flooding and water-energy challenges , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13868, https://doi.org/10.5194/egusphere-egu25-13868, 2025.

EGU25-16365 | ECS | Posters on site | ITS1.3/NP0.2

Redefining Urban Clusters: Combining Subjective Perceptions and Objective Data to Map Inequality 

Shubham Pawar, Tony Robertson, Armando Marino, and Craig Anderson

In recent decades, inequalities in economic, health, and education sectors have intensified spatial clustering of populations and resources, further reinforcing disparities within urban environment. Identifying these geographic boundaries is crucial for developing targeted policies to address inequality effectively. While traditional approaches to studying urban segregation rely primarily on socioeconomic indicators, this research introduces a novel methodology that combines subjective perceptions of the urban environment and objective characteristics of urban areas—such as land use and infrastructure—to identify distinct spatial clusters within Glasgow, a city with a varied socioeconomic landscape. Using MIT Place Pulse dataset of crowd-sourced streetscape perceptions, we developed a deep learning model to predict perception scores for new areas. These perception scores, along with image embeddings and land use information, enabled the geographic clustering of areas based on perceived and functional similarities. Our analysis reveals that perception-based boundaries often diverge from traditional census dissemination areas, suggesting that administrative boundaries may not fully capture the lived experiences of urban space. This research advances our understanding of urban inequality by demonstrating how perceived environmental qualities interact with physical infrastructure to shape distinct urban zones, providing policymakers with new tools for targeted intervention strategies.

How to cite: Pawar, S., Robertson, T., Marino, A., and Anderson, C.: Redefining Urban Clusters: Combining Subjective Perceptions and Objective Data to Map Inequality, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16365, https://doi.org/10.5194/egusphere-egu25-16365, 2025.

The rapid expansion of urban areas has led to significant environmental changes, most notably the Urban Heat Island (UHI) phenomenon, characterized by higher temperatures in urban areas compared to their rural counterparts. Addressing and mitigating UHIs is vital for public health, energy demand management, and enhancing urban livability, especially amidst global climate change. This study focuses on classifying Local Climate Zones (LCZs) in Taipei, Taiwan, using digital building data, satellite imagery, and urban morphological indices. LCZs offer a standardized framework to analyze urban morphology and its influence on local climates. By applying unsupervised clustering methods, we achieved a detailed classification of urban areas, enabling a data-driven exploration of their climatic and morphological characteristics.

To downscale and refine the analysis at the community level, Principal Component Analysis (PCA) was employed to reduce data dimensionality and extract key features such as building coverage, vegetation index, and sky view factor. K-means clustering was then used to categorize urban morphological types, resulting in distinct LCZs across Taipei. Our findings reveal significant differences in environmental variables among clusters. These results highlight how urban morphology, including building density and vegetation cover, impacts local climate conditions. The study also emphasizes the role of thermal comfort, underscoring the complex interplay between urban form and environmental factors.

This research demonstrates the effectiveness of unsupervised classification methods in identifying urban climate zones and provides a practical framework for urban planning and climate adaptation. By enabling targeted interventions, such as greening strategies or ventilation optimization, the study contributes to enhancing urban sustainability and resilience. The findings underscore the importance of interdisciplinary approaches to address the multifaceted challenges of urbanization and climate change.

How to cite: Chen, W.-J., Juang, J.-Y., and Chien, S.-S.: Self-Organizing Local Climate Zones by Using Integrated information in Urban Community – a case study in DaXue Village, Taipei, Taiwan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17835, https://doi.org/10.5194/egusphere-egu25-17835, 2025.

Urban thermal environment is known to be strongly affected by the composition of urban land cover, with densely built-up areas characterised with distinctly higher temperatures than densely vegetated ones. These observations come from the analysis of relatively coarse land surface temperature (LST) satellite data and conclusions are typically derived for city districts or other variedly defined mapping units. Whilst these analyses provide useful insights to excess heat mitigation at city scales, these do not describe the nuance of the thermal response of the heterogenous urban form at local levels. This study investigated the relationship between LST of variedly configured immediate neighbourhoods of single patches of different land cover types (buildings, paved, grass, trees) extending from 0 to 100m away to determine the shape and type of urban features including water that contribute to the formation of cold and hot urban spaces. The study area comprised three English towns: Milton Keynes, Bedford, and Luton, collectively comprising a wide range of urban forms that are representative for England and other European towns located in the temperate climate zone. The analysis was carried out for two summer days a month apart, capturing the different thermal responses as temperatures rise over summer.  The microscale of the analysis was enabled by downscaled LST obtained from Landsat 8 thermal bands acquired at 100m resolution down to 2m, supported by high resolution spectral indices derived from very high resolution hyperspectral aerial imagery. Patch-level landscape metrics were used to describe the shape of the different patches of urban land cover derived from land cover map at 2m resolution. K-means analysis was used to determine groups of land cover patches of a given type with common thermal and spatial properties. Random forest regression algorithm was used to identify the important descriptors of LST for these groups and ANOVA analysis to determine statistically significant effects for various spatial configuration metrics. The findings suggested that the coldest patches of buildings, grass and paved were associated with highly aggregated patches of trees in the immediate neighbourhood, with PLADJ greater than 73 to 85% and COHESION greater than 93 to 97%, and buildings requiring somewhat lower aggregation levels than grass or paved. Hottest patches of these land cover classes were associated with PLADJ smaller than 63–69% and COHESION smaller than 83–87%, with elevation and distance to water being the most important factors, whose importance increased as the summer progressed. Overall, this study provided further insights into the spatial characteristics of patches of common land cover types in urban areas that contribute to the formation of particularly hot or cold urban spaces, which can facilitate the design of climate resilient cities.

How to cite: Zawadzka, J., Harris, J., and Corstanje, R.: The importance of spatial configuration of urban form in local temperature regulation investigated from very high resolution LST and land cover data and landscape metrics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19759, https://doi.org/10.5194/egusphere-egu25-19759, 2025.

EGU25-20244 | ECS | Posters on site | ITS1.3/NP0.2

Comparing the effectiveness of Landsat-derived spectral indices for building age prediction in urban energy modelling 

Thomas Vigato, Letizia Dalle Vedove, Camilla Dalla Vecchia, Claudio Zandonella Callegher, and Samuele Zilio

The building stock accounts for 34% of global energy demand and 37% of CO₂ emissions related to energy and industrial processes. Additionally, the current increase in urbanization rates poses significant environmental challenges. Policy makers are becoming increasingly aware of these impacts, developing strategies aimed at improving energy efficiency and obtaining decarbonization of the built environment. Achieving these goals requires modeling actual building stock energy consumption patterns, future energy developing trends as well as the impact of energy retrofitting measures on CO₂ emissions. Urban Building Energy Models (UBEMs) and bottom-up engineering models have proven to be valuable tools. However, these models  require detailed and accurate building attributes related to physical properties (building geometry, height, building type, thermal transmittances, etc.), local climate (air temperature, humidity, solar radiation, etc.) and data related to occupants' energy behavior (occupants’ schedule, heating and cooling energy demand, efficiency of the system etc.). Among others, building construction year is one of the most relevant parameters since it is a key proxy for essential characteristics such as morphology, facade design, building materials, and energy efficiency. However, obtaining building construction year is particularly challenging as it is rarely available in public databases and, when available, the data are often incomplete or inconsistent. In this regard, remote sensing techniques can play a crucial role in the study and monitoring of the building stock. In particular, satellite images represent an excellent tool for the estimation of building age at local or regional scale given their extensive temporal and spatial coverage, as well as and the continuous updates of collections. The study focuses on the city of Parma, for which seven images covering the year range between 1985 and 2011 were selected. After a literature review, five built-up area extraction indices suitable for TM sensor were selected: Normalized Difference Built-up Area Index (NDBI), New Built-up Index (NBI), Band Ratio for Built-up Area (BRBA), Normalized Built-up Area Index (NBAI), and Vegetation Index Built-up Index (VIBI). In addition, Normalized Difference Vegetation Index (NDVI) was also considered, leading to a total of six indices. To improve the ability of these indexes to discriminate urban surfaces from areas with similar spectral signature (bare soil, sand, rock, etc.) annual greenest pixel composite images were generated using Google Earth Engine. Indexes performance was then compared on each image evaluating Receiver Operating Characteristic (ROC) and Precision-Recall (PR) curves, as well as performance metrics such as F1-score and Area Under the Curve (AUC). The results indicate that the NDVI is the best- Finally, temporal series were derived from the classification of images from different years, enabling the assessment of urbanization growth over time and, consequently, the estimation of building ages.

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) – SPOKE TS 1

 
 
 

How to cite: Vigato, T., Dalle Vedove, L., Dalla Vecchia, C., Zandonella Callegher, C., and Zilio, S.: Comparing the effectiveness of Landsat-derived spectral indices for building age prediction in urban energy modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20244, https://doi.org/10.5194/egusphere-egu25-20244, 2025.

EGU25-821 | ECS | Posters on site | ITS4.1/NP0.3

Development and Validation of a Tipping Element Emulator Integrated into a Simplified Climate Model to Simulate the AMOC Collapse 

Amaury Laridon, Victor Couplet, Wim Thiery, and Michel Crucifix

Despite its potential future collapse and profound impacts, assessing the tipping dynamics of the Atlantic Meridional Overturning Circulation (AMOC) remains a significant challenge. Complex models such as Earth System Models (ESMs) and Earth System Models of Intermediate Complexity (EMICs) introduce substantial uncertainties in identifying tipping points. To address this, recent research has focused on developing conceptual models based on non-linear dynamics to capture the tipping behavior of the system. However, existing conceptual models typically simulate the AMOC response to a single temperature forcing, whereas it is well established that the AMOC is also influenced by freshwater flux.

In this study, we develop and validate an AMOC Tipping Calibration module that incorporates two forcing parameters: global mean temperature and freshwater flux. This module is designed as an emulator for the AMOC response within cGenie, an EMIC. Following validation, the emulator is integrated into SURFER, a simplified climate model that enables rapid and efficient simulations of AMOC trajectories under various scenario-based pathways. Our results show that incorporating both forcing parameters improves the accuracy of AMOC trajectory predictions. The methodology used to develop the two-parameter emulator is generalizable and can be applied to other tipping elements. By facilitating a greater number of simulations than complex models while maintaining calibration to them, this tool represents a significant advancement in exploring and understanding the potential future behaviour of the AMOC and other tipping elements.

How to cite: Laridon, A., Couplet, V., Thiery, W., and Crucifix, M.: Development and Validation of a Tipping Element Emulator Integrated into a Simplified Climate Model to Simulate the AMOC Collapse, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-821, https://doi.org/10.5194/egusphere-egu25-821, 2025.

EGU25-859 | ECS | Orals | ITS4.1/NP0.3 | Highlight

Reconciled warning signals in observations and models indicate a nearing AMOC tipping point  

Yechul Shin, Ji-Hoon Oh, Niklas Boers, Sebastian Bathiany, Marius Årthun, Huiji Lee, Tomoki Iwakiri, Geon-Il Kim, Hanjun Kim, and Jong-Seong Kug

The Atlantic Meridional Overturning Circulation (AMOC), as recorded in paleoclimate proxies, is one of the climate systems with a potential abrupt transition. Increasing identification of statistical signals—critical slowing down—in observational fingerprints empirically raises concerns that the system may be approaching a tipping point. However, state-of-the-art Earth System Models (ESMs) rarely project an abrupt collapse of AMOC, and its loss of stability has yet to be thoroughly investigated, leaving it unclear whether warning signals of AMOC tipping is overlooked in ESMs or exaggerated in fingerprints. Here, a warning signal over the deep convection site of AMOC is consistently identified in both observations and ESM, and we present that the currently observed signal is reconciled with the modeled one, with warming exceeding the Paris Agreement goal. This warning signal is in accordance with physical stability of the AMOC, the AMOC-induced freshwater convergence into the Atlantic basin, is overestimated in the ESM, so that it projects a delayed tipping point. These results suggest that the observed AMOC is approaching a tipping point akin to the projections of models simulating a much warmer Earth, underscoring potentially overlooked risks in ESMs assessments.

How to cite: Shin, Y., Oh, J.-H., Boers, N., Bathiany, S., Årthun, M., Lee, H., Iwakiri, T., Kim, G.-I., Kim, H., and Kug, J.-S.: Reconciled warning signals in observations and models indicate a nearing AMOC tipping point , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-859, https://doi.org/10.5194/egusphere-egu25-859, 2025.

In this paper, I explore how to assess technologies’ potential to aid a sustainable transformation via societal tipping points. I do this by providing a definition of sustainability that combines justice, well-being, and the value of nature with insights from value-sensitive design and the technology assessment literature. This exploration serves as an additional consideration for the developing societal tipping point scholarship. I argue that research surrounding societal tipping points can be meaningfully bolstered through philosophical reflection on the inherent ethical implications of sustainability, and the value-ladenness of technological development. There is a salient push within various strands of climate adaptation and sustainable transition scholarship towards systems thinking. In order to reorient society within the Anthropocene, and to adapt to a destabilized climate, such scholarship argues that the underlying subsystems society currently relies on need to change. Conceiving societal structures, such as institutional, political, and financial arrangements, the various planetary spheres (bio-, cryo-, hydro-, atmo-, and geosphere), and the techno-scientific infrastructure as interdependent systems has heuristic and practical allure. As a heuristic, it allows researchers and policymakers to account for the numerous interrelated systems that affect climate change and environmental degradation. Practically, this heuristic should enable the identification of impactful and sustainable action. Knowing how the subsystems interoperate, what drives them, and what function they provide, accordingly serves as a baseline to identify possible leverage points to change them. Conceptually mirroring climate tipping points, there is growing interest in societal tipping points as possible catalysts for decisive climate action. This interest is premised on the idea that societal tipping points within a currently unsustainable global societal-ecological-technical system can be identified and operationalized in order to tip the system (or subsystems) into a sustainable direction This premise raises at least two critical issues that have so far received little attention. First, the question arises what tipping towards a more sustainable system would look like. The concept of sustainability is arguably vague, especially when it comes to its aptness in describing climate action. Answering this question requires a reflective and ethically thick conception of sustainability, which in turn, needs to represent a future-oriented conception of justice, well-being, and nature. Second, it is crucial to reflect on the interdependent ways in which technological development and the implementation of new technologies affect the societal values and norms that drive them, since technology plays a central role for achieving societal tipping points. If technology is seen as a an accelerator and facilitator for a sustainable transition, the value-ladenness that technological innovation comes with needs to be addressed. Importantly, some technologies that seem sustainable on the surface, may actually entrench and enforce existing unsustainable modes of behavior and policies. Accordingly, this paper expands on the societal tipping points literature by proposing a concept of sustainability that serves as a means to assess the potential of technologies to facilitate sustainable tipping.

How to cite: Hofbauer, B.: Can We Tip Sustainably? Ethical Considerations on the Role of Sustainable Technology in Societal Tipping Points, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2923, https://doi.org/10.5194/egusphere-egu25-2923, 2025.

EGU25-3514 | ECS | Orals | ITS4.1/NP0.3

Critical Salinity as an early warning of Tipping Point in the North Atlantic Subpolar Gyre 

Lucas Almeida and Didier Swingedouw

The subpolar gyre (SPG) of the North Atlantic plays a pivotal role in the Atlantic Meridional Overturning Circulation (AMOC) and climate through various teleconnections. This study examines the tipping point in thisregion within CMIP6 projections using three models: CESM2-WACCM, MRI-ESM2-0, and NorESM2-LM. These models, selected for exhibiting tipping patterns in at least one emission scenario, reveal distinct yet converging patterns of change, suggesting a destabilization of the subpolar region driven by shifts in salinity, temperature, and density profiles. A consistent feature across the models is pronounced freshening in the upper 150 meters of the water column. This results in a strong stratification, accompanied by cooling in the top 250 meters and warming between 150 and 1500 meters. The resulting enhancement in water column stability leads to a marked reduction in mixed layer depth (MLD). These changes disrupt vertical mixing, weaken nutrient transport, and alter regional circulation dynamics, with cascading effects on marine ecosystems and climate feedback mechanisms. We employed a density-based approach that accounts for the combined effects of temperature and salinity on water density to identify the critical surface salinity leading to the tipping of the SPG. This critical salinity represents a threshold for the salinity level beyond which density-driven stratification results in a stable water column. For stability to break, surface salinity must exceed this critical salinity. All three models consistently identify a critical salinity threshold of approximately 33.8 g·kg⁻¹. When surface salinity drops below this threshold, the subpolar region experiences rapid cooling, reduced convection, and potentially irreversible transitions. The tipping point of the SPG is preceded by an expansion of areas in the SPG where surface salinity falls below this critical threshold, accompanied by a decrease in MLD. To complement our analyses, we used the ISAS dataset to assess how far the system is from an SPG tipping point. Our next step is to establish an observable spatial pattern of early warning. Our findings underscore the vulnerability of the North Atlantic subpolar region to salinity-driven tipping points, which may lead to potentially irreversible transitions. This highlights the critical need for precise monitoring and advanced modeling of salinity dynamics to enhance predictability in future climate scenarios.

How to cite: Almeida, L. and Swingedouw, D.: Critical Salinity as an early warning of Tipping Point in the North Atlantic Subpolar Gyre, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3514, https://doi.org/10.5194/egusphere-egu25-3514, 2025.

EGU25-3532 | ECS | Orals | ITS4.1/NP0.3

Social norms and groups structure safe operating spaces and exhibit regime shifts in renewable resource use in a social-ecological multi-layer network model 

Max Bechthold, Wolfram Barfuss, André Butz, Jannes Breier, Sara Constantino, Jobst Heitzig, Luana Schwarz, Sanam Vardag, and Jonathan Donges

Social norms are a key socio-cultural driver of human behaviour and have been identified as a central process in potential social tipping dynamics. They play a central role in governance and thus represent a possible intervention point for collective action problems in the Anthropocene, such as natural resource management. 
A detailed modelling framework for social norm change is needed to capture the dynamics of human societies and their feedback interactions with the natural environment. To date, resource use models often incorporate social norms in an oversimplified manner, as a robust and detailed coupled social-ecological model, scaling from the local to the global World-Earth scale, is lacking. 
Here we present a multi-level network framework with a complex contagion process for modelling the dynamics of descriptive and injunctive social norms. The framework is complemented by social groups and their attitudes, which can significantly influence the adoption of social norms. We integrate the modelling concept of norms together with an additional individual social learning component into a model of coupled social-ecological dynamics with a closed feedback loop, implemented in the copan:CORE framework for World--Earth modelling.
We find that norms generally bifurcate the behaviour space into two extreme states (sustainable vs. unsustainable) divided by regime shifts. Reaching a sustainable (i.e. safe) state becomes more likely with low thresholds of conforming to sustainable norms, as well as lower consideration rates of own resource harvesting success. The success of a generic social norm intervention is also found to be highly dependent on the group topology and exhibit a phase-transition like shape under certain conditions. The regime shifts in thresholds, individual learning and norm intervention hint at exploitable underlying tipping processes.
Our findings suggest that explicitly modelling social norm processes together with social groups enriches the dynamics of social-ecological models and determines safe operating spaces. Consequently, both should be taken into account when representing human behaviour in coupled World--Earth models.

How to cite: Bechthold, M., Barfuss, W., Butz, A., Breier, J., Constantino, S., Heitzig, J., Schwarz, L., Vardag, S., and Donges, J.: Social norms and groups structure safe operating spaces and exhibit regime shifts in renewable resource use in a social-ecological multi-layer network model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3532, https://doi.org/10.5194/egusphere-egu25-3532, 2025.

EGU25-6613 | Posters on site | ITS4.1/NP0.3

Spatial variance and spatial skewness as leading indicators of regime shifts in global forests 

Matteo Mura, Deepakrishna Somasundaram, Mirco Migliavacca, Vasilis Dakos, Alessandro Cescatti, and Giovanni Forzieri

Forests have considerable potential to influence the stability of the Earth system and mitigate climate change by influencing biogeochemical and biophysical processes. Tree cover, as the primary layer of exchange for carbon, energy and water cycles, play a critical role in such dynamics. However, the persistence and functionality of forests are highly dependent on their resilience to the ongoing rapid changes in natural and anthropogenic pressures. Experimental evidence of a sudden increase in tree mortality across different biomes is rising concerns about the ongoing changes in forest resilience and the associated risks to the climate mitigation potential of forests. Previous global-scale assessments of forest resilience have focused on the use of critical slowing down indicators, such as temporal autocorrelation and variance. These studies have provided important insights, but they can only partially capture the effects of stochastic disturbances and forest management.  

In this study, we explore the potential of spatial statistical indicators (SSI), such as spatial variance and skewness, as early warning signals of regime shifts in global forests. To this aim, we first derive tree cover values for the 2000-2023 period at 0.05-degree spatial resolution for the whole globe by combining multiple satellite observations. We then, develop a machine learning model to disentangle the climate effects on tree cover distributions and elucidate the underlying mechanisms. SSI are ultimately computed on the residuals of the machine learning model and their spatial and temporal variations analysed.

Results show, along with a widespread erosion of tree cover, an increase in both SSI prominently in tropical and boreal forests over the observational period. According to the stability theory, the simultaneous increase in these metrics indicates a rising instability of the system by reflecting an alteration of the shape of the basin of attraction. Such patterns appear largely driven by the increase in stochastic perturbations and human pressures which are not detected using traditional critical slowing down indicators. Overall, this study contributes to better understand the recent dynamics in forest resilience and its underlying mechanisms that can lead to critical transitions. Considering the expected intensification of natural pressures in view of climate change, it is becoming urgent to identify adaptation measures to preserve the long-term stability of global forests and the provision of their ecosystem services.

How to cite: Mura, M., Somasundaram, D., Migliavacca, M., Dakos, V., Cescatti, A., and Forzieri, G.: Spatial variance and spatial skewness as leading indicators of regime shifts in global forests, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6613, https://doi.org/10.5194/egusphere-egu25-6613, 2025.

EGU25-7369 | Orals | ITS4.1/NP0.3

Detection of global-scale tipping using climate networks  

Maura Brunetti, Jérôme Kasparian, and Laure Moinat

The climate system is prone to various tipping mechanisms at the global scale, such as the abrupt changes induced by the potential shutdown of the Atlantic meridional overturning circulation. Thus, it is essential to develop robust Early Warning Signals (EWSs) to assess the risk of crossing tipping points. Classically, EWSs are statistical measures based on time series of climate state variables, and their spatial distribution is not exploited. However, spatial information is crucial to identifying the starting location and development of a transition process. Methods that use spatial information become particularly relevant in the current era, when satellite observations with high spatiotemporal coverage produce huge amounts of data.

We use complex networks constructed from several climate variables (like surface air temperature, specific humidity and cloud cover) on the numerical grid of climate simulations. Using the pyUnicorn Python package [1], we construct networks based on linear and nonlinear spatial correlations of time series at each grid point. We seek for network properties that can serve as EWS when approaching a state transition at the planetary scale, as obtained by the MIT general circulation model in a coupled-aquaplanet configuration for CO2 concentration-driven simulations.

We show that network indicators such as the normalized degree, the average length distance and the betweenness centrality are capable of detecting tipping points at the global scale [2]. We assess and compare the applicability as EWS of these indicators to traditional methods. Moreover, we analyse climate networks’ ability to identify nonlinear dynamical patterns. Finally, we discuss the generalisation to network indicators that include causal relationships.

References

[1] J. Donges et al., Unified functional network and nonlinear time series analysis for complex systems science: The pyunicorn package, Chaos 25, 113101 (2015)

[2] L. Moinat, J. Kasparian, M. Brunetti, Tipping detection using climate networks, Chaos 34, 123161 (2024)

How to cite: Brunetti, M., Kasparian, J., and Moinat, L.: Detection of global-scale tipping using climate networks , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7369, https://doi.org/10.5194/egusphere-egu25-7369, 2025.

EGU25-10019 | Orals | ITS4.1/NP0.3

Optimal climate policies under the shadow of social tipping 

Michael Kuhn, Gernot Wagner, and Stefan Wrzaczek

We propose a framework that allows to integrate social (tipping) dynamics into a DICE-style IAM model, in which a policy maker determines abatement effort and savings. The policy maker maximizes the sum of social welfare and a political penalty/reward, depending on whether the majority of the population opposes (penalty) or supports (reward) more ambitious abatement policies. The social process itself depends inter alia on observable climate impacts. We provide numerical simulations that illustrate the impact of the tipping process on policy choices which in turn are built around a total cost of carbon that embraces both the "classical" social cost of carbon and a political cost of carbon. Our initial findings illustrate (i) the considerable scope for political penalties (rewards) to stifle (boost) abatement policies; (ii) an incentive for the policy maker to distort policies in a way that boosts political support; and (iii) a considerable deviation between the total cost of carbon and the social cost of carbon. We argue how the model can be used for the purpose of understanding climate policy making from a "social dynamics" perspective.

How to cite: Kuhn, M., Wagner, G., and Wrzaczek, S.: Optimal climate policies under the shadow of social tipping, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10019, https://doi.org/10.5194/egusphere-egu25-10019, 2025.

EGU25-10648 | ECS | Orals | ITS4.1/NP0.3

Assessing the Probability of CO2-Driven AMOC Collapses Using Rare Event Algorithms in PlaSIM-LSG 

Matteo Cini, Valerian Jacques-Dumas, and Henk A. Dijkstra

The Atlantic Meridional Overturning Circulation (AMOC) is a key tipping element of the climate system due to its influence in regulating the meridional transport of heat and freshwater. Its stability is influenced by the interplay between external forcings (such as greenhouse gasses increase) and internal climate variability. Due to limitations on the deterministic predictability of the AMOC asymptotic state, the concept of a “probabilistic safe operating space” has been proposed. For this purpose, rare-event techniques, specifically the Giardina–Kurchan–Tailleur–Lecomte (GKTL) and Trajectory-Adaptive Multilevel Splitting (TAMS) algorithms, offer promising tools for testing the multistability of the system and assessing this probability at lower computational costs than traditional Monte Carlo methods.  Here, using the intermediate complexity model (PlaSIM-LSG), we estimate the probability of AMOC collapse in sensitivity experiments at different CO2concentrations and under RCPs scenarios. In particular, TAMS has been applied in order to assess the probability of reaching a low circulation state of the AMOC associated with a 1°C temperature anomaly over central and western Europe. Our findings from sensitivity experiments, consistently with previous studies, indicate that for a wide range of CO2 concentrations (500-600 ppm), the probability of an AMOC collapse is significantly different from zero (1-10% within 150 years). While such a collapse is unlikely to happen within the 21st century, it becomes likely to happen by 2150 in higher emission scenarios. It is important to note that PlaSIM-LSG does not account for the North Atlantic freshwater flux from Greenland melting which introduces a stabilizing bias for the AMOC-on state. Accounting for this mechanism would likely increase the probability of an AMOC collapse. These results underscore the importance of probabilistic assessments in understanding AMOC stability and highlight the potential for rare-event algorithms to provide insights into the statistical properties of tipping point.



How to cite: Cini, M., Jacques-Dumas, V., and Dijkstra, H. A.: Assessing the Probability of CO2-Driven AMOC Collapses Using Rare Event Algorithms in PlaSIM-LSG, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10648, https://doi.org/10.5194/egusphere-egu25-10648, 2025.

EGU25-10788 | ECS | Orals | ITS4.1/NP0.3

Manifesting tipping points in pro-environmental behaviour for climate change mitigation 

Thomas Elliot, Jonathan Donges, Massimo Pizzol, and Ilona Otto

Achieving ambitious climate change targets, such as limiting global warming to 1.5°C, requires both political and social determination. Bottom-up pro-environmentalist behaviours can facilitate crossing social tipping points (STPs), resulting in new social norms with lower impact on global warming. While the passing of  STPs has been described qualitatively, it remains poorly understood how the climate benefits of this phenomenon can be quantified. 
Here, we introduce a stylised system dynamics model that couples socio-ecological contagion with global warming via greenhouse gas emission pathways to estimate the impact of crossing social tipping points on greenhouse gas mitigation and global warming. . This is explored through two examples of bottom-up and top-down mitigation interventions.
Results indicate that a STP could be crossed before 2050. While neither bottom-up nor top-down interventions alone are likely to achieve the 1.5°C target, their combined effect significantly reduces overshoot. This represents a significant step towards understanding how both bottom-up and top-down interventions can be harnessed to mitigate global warming. Our research underscores the importance of bottom-up pro-environmental movements, emphasizing their crucial role in not only reducing personal carbon footprints but also alleviating the burden on technological top-down interventions. This evidence of the benefits of promoting socio-ecological contagion should bolster the determination of individuals and community grassroots groups. Additionally, it should encourage top-down interventions to acknowledge and support the complementary role of collective action.

How to cite: Elliot, T., Donges, J., Pizzol, M., and Otto, I.: Manifesting tipping points in pro-environmental behaviour for climate change mitigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10788, https://doi.org/10.5194/egusphere-egu25-10788, 2025.

EGU25-10947 | ECS | Orals | ITS4.1/NP0.3

Causal effect estimation for robust detection of critical slowing down 

Alexandrine Lanson and Jakob Runge

A tipping element is a system that may pass a tipping point, that is, a threshold value of an environmental stressing condition at which a small disturbance can cause an abrupt shift of the tipping element from one state to another, accelerated by positive feedbacks. For example, under rising temperatures and increasing deforestation, the Amazon rainforest could tip from a forest state to a savanna state; one feedback involved is that fewer trees means less evapotranspiration, thus less rainfall and, finally, less trees. Therefore, the fewer trees, the harder it is for the remaining forest to adapt and survive. This phenomenon is called critical slowing down: approaching a bifurcation, a tipping system's resilience decreases, resulting in increasing autocorrelation and variance. The latter indicators are thus often measured to detect bifurcation-induced tipping and are called early-warning signals (EWS).

Let us describe the dynamics of a tipping element Y with the following equation: dY/dt = f(Y, r) + η, with r the environmental stressing condition involved in the tipping behavior and η some noise (e.g., climate variability). Deriving EWS directly from Y's time series relies on the assumption that the noise η is not correlated (white-noise), otherwise any trend in η's autocorrelation would be incorporated in Y's autocorrelation, even if not related to the tipping behavior contained in f(Y, r). In the Amazon rainforest example, increasing deforestation due to human activity is a part of r with a long-term effect, while e.g. ENSO also influences the forest but on short time scales and with sometimes opposite effects depending on its phase (El Niño/La Niña/neutral), and would be part of η.  If for example El-Niño's autocorrelation increases with time, the rainforest autocorrelation might also increase regardless of whether the forest is approaching the bifurcation point or not, therefore the autocorrelation would no longer reflect changes in the forest resilience.

To know how far the system is from the bifurcation point, we want to measure Y's internal autocorrelation (excluding noisy influences η, considering only f(Y, r)), and thus to answer the question: "If we intervene in the system and set the value of Y at time t-1, how does Y evolve at time t?" This defines the direct causal effect of Yt-1 on Yt and comes under the heading of causal inference: we look at the influence of setting Yt-1=yt-1 on Yt, whatever the values of the other variables causing Y, which is fundamentally different from a direct measure where the value of Y at time t-1 is, in the general case, dependent on the state of the other variables. To measure how the direct causal effect of Yt-1 on Yt  evolves with time (with changing r), we use causal effect estimation, which quantifies the causal effect of hypothetical interventions in a system from observational data --the interventional distribution being rarely available in the majority of systems--- and an assumed causal graphical model that allows us to derive an adjustment expression that controls for confounders. We demonstrate the method on an ideally forced simulated system and discuss potential applications.

How to cite: Lanson, A. and Runge, J.: Causal effect estimation for robust detection of critical slowing down, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10947, https://doi.org/10.5194/egusphere-egu25-10947, 2025.

EGU25-11175 | ECS | Posters on site | ITS4.1/NP0.3

Tipping the AMOC: Impacts of Tropical Cyclones in a Changing Climate 

Nicolas Colombi, Chahan M. Kropf, Friedrich A. Burger, Simona Meiler, Kerry Emanuel, Thomas L. Frölicher, and David N. Bresch

The Atlantic Meridional Overturning Circulation (AMOC) is one of the most critical tipping elements in Earth’s climate system, with its collapse posing far-reaching implications for weather dynamics and extremes, sea level rise, and Northern Hemisphere cooling. Although it is considered a low-probability but high-impact scenario, recent studies suggest that the AMOC may already be on a trajectory towards collapse. Moreover, current climate models struggle to fully capture the complex interactions between Greenland ice sheet melting and the AMOC slowdown, adding further uncertainty to climate projections. Artificial hosing experiments in the North Atlantic, project the weakening of the AMOC to increase sea surface temperature in the Southern Hemisphere and the tropics, particularly in ocean basins where tropical cyclones form. This warming, combined with rising sea levels and changes in vertical wind shear, could create conditions that promote the development of tropical cyclones and amplify their impacts. Although several studies have explored the relationship between tropical cyclone activity and AMOC weakening, the associated socioeconomic impacts remain uncertain. The goal is to investigate the direct and indirect socioeconomic impacts of tropical cyclones under future climate scenarios characterized by a weakened and fully collapsed AMOC. Will tropical cyclones affect areas that were previously unaffected? Will tropical cyclones' activity intensify, leading to greater societal impacts? To answer these questions, two sets of five-member ensemble simulations were performed for a 2°C stabilization emission scenario using the GFDL ESM2M, with and without induced AMOC collapse. These simulations were then coupled with the MIT coupled statistical-dynamical tropical cyclone model to simulate tropical cyclone activity under these conditions, and the probabilistic climate risk modeling platform CLIMADA was used to analyze the socioeconomic impacts. We anticipate this study to be a stepping stone in a broader ongoing effort to assess the socioeconomic impacts of extreme weather events triggered by tipping points.

How to cite: Colombi, N., Kropf, C. M., Burger, F. A., Meiler, S., Emanuel, K., Frölicher, T. L., and Bresch, D. N.: Tipping the AMOC: Impacts of Tropical Cyclones in a Changing Climate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11175, https://doi.org/10.5194/egusphere-egu25-11175, 2025.

EGU25-12221 | Posters on site | ITS4.1/NP0.3

Challenges and solutions on identification of high-performance black plastics for closed-loop car recycling   

Andréa de Lima Ribeiro, Margret Fuchs, Yuleika Madriz, and Richard Gloaguen

Plastics represent, in volume, up to 50% of materials present in modern vehicles with most of them being black. Consequently, black plastics are a key material stream to be managed in end-of-life vehicles (ELV) waste. The EU directive on ELV, updated in 2023, introduces new rules covering all aspects of a vehicle life cycle, from its design and market placement until its final treatment as ELV. These new specific criteria now put pressure on car manufacturers and black plastic recyclers to boost circularity in the production and recycling chains, including:

  • Improving circular design of vehicles to facilitate removal of materials, parts and components for reuse and recycling;
  • Ensuring that at least 25% of the plastics used to build a new vehicle comes from recycling (of which 25% from recycled ELVs).

The first step required to improve the circularity of ELV polymers is to identify the main polymer types present in the stream with optical sensing. Current identification workflows are successfully employed by the plastic-waste recycling industry, based on material-specific signals present in the visible-to-near infrared (VNIR) and short-wave infrared (SWIR) ranges (400–2500 nm). Nevertheless, VNIR/SWIR sensors are unsuitable for identification of black plastics due to the strong signal absorption by dark pigments in this spectral region. In recent years, novel hyperspectral sensors operating in mid-wave infrared (MWIR, 2700–5300 nm) have been successfully employed for identification of black plastics. Yet, the automotive industry requires high-performance materials which led to the development and use of very specific polymer variants, including multi-polymer blends (e.g. ABS/PC), polymer subtypes (e.g. PA6 and PA6.6), and functional additives (e.g. glass fiber, talc, carbon black). Consequently, the identification of the usual polymer classes is not adapted to meet the minimum quality requirements for recycling and, hence, not adequate for future use for car material streams (closed loop). 

Such complexity is justified by the need for high performance and functionality of materials in automotive applications, but impacts recyclability and ultimately leads to downcycling. In order to ensure that high-purity black plastics are obtained at the end of the recycling operation, at the standards needed by the automotive industry, it is necessary to go beyond the identification of main polymer types. 

In this contribution, we address the current challenges and propose solutions to identify the important high-performance polymers used by the automotive industry that could be recycled. Further, we evaluate the suitability of current industrial optical sensing techniques for identification of black plastics originated from ELV waste. We also propose solutions for the identification of plastics with highly-complex composition present in ELVs such as multi-polymer blends (e.g. ABS/PC), polymer subtypes (e.g. PA6 and PA6.6), and functional additives (e.g. glass fiber, talc, carbon black).

How to cite: de Lima Ribeiro, A., Fuchs, M., Madriz, Y., and Gloaguen, R.: Challenges and solutions on identification of high-performance black plastics for closed-loop car recycling  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12221, https://doi.org/10.5194/egusphere-egu25-12221, 2025.

EGU25-13560 | Posters on site | ITS4.1/NP0.3

Vegetation resilience and sensitivity in complex dynamic vegetation models 

Sebastian Bathiany, Lana Blaschke, Andreas Morr, and Niklas Boers

Resilience is typically defined as the ability of vegetation to recover from external perturbations such as fires or droughts, and it can be quantitatively measured by the rate of recovery following such events. Resilience can also be assessed indirectly, even in the absence of large perturbations. One key metric for this is autocorrelation. A loss of resilience over time, often referred to as "slowing down," can be detected as an increase in autocorrelation. In simple one-dimensional dynamical systems, a reduction in resilience is also associated with increased sensitivity of the system's stable state to external conditions.

Recent studies, using indicators such as the Normalized Difference Vegetation Index (NDVI) and Vegetation Optical Depth (VOD), have found that resilience tends to be higher in wetter regions of tropical forests compared to drier regions, and that resilience has been decreasing across large parts of the Amazon rainforest. Additionally, empirical recovery rates after disturbances have been found to correlate with autocorrelation, supporting the practical relevance of theoretical expectations. However, it remains unclear which specific vegetation properties and processes determine the observed patterns.

Here we use idealized simulations with the state-of-the-art dynamic vegetation model LPJmL and explore how the resilience of natural forests and its indicators depend on (i) climate, (ii) vegetation composition (i.e., the mix of plant functional types), (iii) the vegetation property (variable) being considered, and (iv) the nature of the perturbation(s). We find that autocorrelation qualitatively aligns with the recovery time from large, negative perturbations that affect all tree types similarly.

However, there are exceptions where the factors listed above can influence the relationship in unexpected ways. Specifically, for some tree types and climate regimes, recovery rates and autocorrelation do not align with each other, nor with the forest's sensitivity to climate change. For example, perturbations that alter the relative abundance of tree types can lead to different recovery rates compared to those affecting all tree types uniformly. Moreover, vegetation variables that recover quickly when perturbed in isolation (e.g., fluxes like net primary productivity) may still co-evolve with slower variables they depend on (e.g., carbon stored in trees). We identify key mechanisms behind these features in the model and test their relevance by simulating a more realistic setup, using observed climate data within a geographically realistic domain. We also discuss the relevance of these mechanisms in the real world.

Our findings highlight the need to better understand the nature of disturbances and trends in ecosystems, as well as the mechanisms captured by satellite-derived indicators. This knowledge, along with improved resilience monitoring, will be crucial for making reliable predictions about how ecosystems will respond to human-induced changes.

How to cite: Bathiany, S., Blaschke, L., Morr, A., and Boers, N.: Vegetation resilience and sensitivity in complex dynamic vegetation models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13560, https://doi.org/10.5194/egusphere-egu25-13560, 2025.

EGU25-13620 | ECS | Posters on site | ITS4.1/NP0.3

Optimizing Plastic Identification in E-Waste Recycling through Hyperspectral Imaging and Transformer-Based Machine Learning Models 

Elias Arbash, Andréa de Lima Ribeiro, Margret Fuchs, Pedram Ghamisi, Paul Scheunders, and Richard Gloaguen

The rapid growth of the electronics market, driven by high demand for new technologies, has shortened the lifespan of electronic products, leading to a surge in electronic waste (E-waste). Comprising 25% plastics, E-waste contains unrecovered critical and toxic materials, necessitating advanced recycling strategies. HeliosLab, an infrastructure combining imaging sensors and robotic chemical analyses, was developed at the Helmholtz Institute Freiberg. HeliosLab integrates spectroscopy-based modalities such as RGB and hyperspectral imaging (HSI) across multiple wavelength ranges that can be used to optimize E-waste sorting. The complexity of the hyperspectral data, compounded by multisensory integration, requires sophisticated automated algorithms to efficiently process large volumes of data and extract critical material features. These advancements ensure scalable, fast, and automated detection solutions for industrial-scale E-waste recycling operations.

We are developing smart and novel processing methodologies utilizing state-of-the-art (SOTA) machine learning hyperspectral imaging (HSI) classification models. In this study, we focus on Transformer-based architectures, known for their self-attention mechanisms that effectively capture contextual relationships between their input tokens, which enables unique spatial-spectral feature detection, relevant to remote sensing and HSI applications. Such an approach significantly advances automated polymer identification. 

To test the model’s performance on unseen data and evaluate the generalization performance of those SOTA models in industrial-like environments, multiscene datasets are required. We acquired a new multiscene HSI polymer dataset in the near visible (NIR) to the short-wave infrared (SWIR) (400-2500 nm) using hyperspectral cameras available at HeliosLab. The initial deployment highlighted the challenges related to both, the data quality and quantity, as well as regarding methodological frameworks. This led us to develop a tailored Transformer-based topology capable of detecting polymer fingerprints using novel refined extractions of the spatial and spectral features. Our research and advancements contribute to the automation and optimization of polymer detection in E-waste recycling, paving the way for improved resource recovery and environmental sustainability.

How to cite: Arbash, E., de Lima Ribeiro, A., Fuchs, M., Ghamisi, P., Scheunders, P., and Gloaguen, R.: Optimizing Plastic Identification in E-Waste Recycling through Hyperspectral Imaging and Transformer-Based Machine Learning Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13620, https://doi.org/10.5194/egusphere-egu25-13620, 2025.

The global climate system continues to change under the influence of human activities. Of particular concern is the difficulty of continuing human activities due to irreversible and long-term abrupt changes caused by the global climate system exceeding its tipping point. Climate systems that have the potential to exceed the tipping point are called tipping elements and are being studied. Among them, the Atlantic Meridional Overturning Circulation (AMOC) plays a central role in the movement of materials through the ocean and is connected to many other tipping elements. While there is concern that the AMOC may decrease in strength due to rising temperatures in the Atlantic Ocean, freshwater inflow due to melting ice in the Arctic region has been investigated as a stabilizing factor. Therefore, it is important to comprehensively consider these influences when evaluating the AMOC tipping point.

 

In the AMOC modelling, Stommel’s two box model describes its nature well. Although, it does not treat freshwater input from multiple estuaries. We have applied three box model (TBM) [1] which divide the Atlantic Ocean into three elements with double estuaries. Freshwater inflows to the Arctic Ocean due to ice sheet thawing in Greenland and permafrost thawing in Siberia were calculated using AWI-ESM [2] and CMIP6 [3] data, respectively. In addition, temperature differences between the southern and northern Atlantic regions were calculated by MRI-ESM2.0 [4].

We also adopted the method of analyzing the time-series behavior of the AMOC as a stochastic process, as in Ditlevsen et al. (2010) [5]. Finally, we estimated the age of AMOC decay based on the analytical AMOC behavior by TBM and by identifying the parameters of the Langevin equation.

 

[1] E. Lambert, T. Eldevik, P.M. Haugan “How northern freshwater input can stabilise thermohaline circulation”, Tellus A: Dynamic Meteorology and Oceanography, 68 (1) (2016), p. 31051

[2] Ackermann, L., Danek, C., Gierz, P., and Lohmann, G. “AMOC Recovery in a multicentennial scenario using a coupled atmosphere-ocean-ice sheet model”, Geophys. Res. Lett., 47, 2020.

[3] Wang, S., Wang, Q., Wang, M., Lohmann, G., & Qiao, F. (2022). ”Arctic Ocean freshwater in CMIP6 coupled models” Earth’s Future, 10(9)

[4] Yukimoto, Seiji; Koshiro, Tsuyoshi; Kawai, Hideaki; et al. (2019) “MRI-ESM2.0 model output prepared for CMIP6 ScenarioMIP ssp585”

[5] Ditlevsen, P. D. and Johnsen, S. J.: Tipping points: Early warning and wishful thinking, Geophys. Res. Lett., 37, L19703, 2010

How to cite: Kono, K. and Fukuda, T.: Instability analysis of the AMOC with varying freshwater input and sea water temperature in the Atlantic Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14805, https://doi.org/10.5194/egusphere-egu25-14805, 2025.

EGU25-15540 | ECS | Orals | ITS4.1/NP0.3

Increased climate tipping risks from temperature overshoots 

Nico Wunderling, Annika Högner, Tessa Möller, Paul Ritchie, Johan Rockström, Norman Steinert, and Jonathan F. Donges

In Paris 2015, the global community agreed to keep global warming well below 2.0°C aiming to limit it to 1.5°C above pre-industrial levels. However, recent research has shown that overshooting this temperature guardrail is becoming increasingly likely and several climate data teams across the world recorded 2024 as the first individual year with a global warming level above 1.5°C.

Such temperature levels endanger critical components of the Earth system, the so-called climate tipping elements such as the Greenland and West Antarctic Ice Sheet, The Atlantic Meridional Overturning Circulation, or the Amazon rainforest. In this presentation, we will show the latest evidence on how overshooting temperature targets increases tipping risks. In particular, we will discuss the role of overshooting the 1.5°C and 2.0°C for the stability of critical Earth system components, and also assess the likelihood for climate tipping cascades beyond these global warming levels.

How to cite: Wunderling, N., Högner, A., Möller, T., Ritchie, P., Rockström, J., Steinert, N., and Donges, J. F.: Increased climate tipping risks from temperature overshoots, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15540, https://doi.org/10.5194/egusphere-egu25-15540, 2025.

EGU25-16872 | ECS | Orals | ITS4.1/NP0.3

The link between topography and climate extinction risks in mountain ecosystems 

Bert Wuyts, Dirk Karger, Jan Sieber, and Victor Boussange

Populations in mountain ecosystems face the risk of extinction due to climate change. Yet, how these risks will materialise remains unclear because many ecological parameters are unknown. We show that progress can be made by examining how habitats get fragmented and isolated as populations shift to higher elevations. When this shift is slow relative to dispersal, the amount of aggregation and connectivity between habitat fragments determine the warming threshold beyond which populations cannot sustain themselves. If the shift is rapid compared to dispersal, there is also a critical warming rate beyond which populations cannot track their preferred range and go extinct. Through simulations and analyses of stochastic spreading processes on real and artificial landscapes, we investigate how mountain topography, warming rates, and demographic mechanisms affect extinction thresholds. Understanding the link between mountain topography and extinction risks may enable targeted interventions to mitigate these risks, especially in areas with fragmentation bottlenecks.

How to cite: Wuyts, B., Karger, D., Sieber, J., and Boussange, V.: The link between topography and climate extinction risks in mountain ecosystems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16872, https://doi.org/10.5194/egusphere-egu25-16872, 2025.

EGU25-16943 | ECS | Orals | ITS4.1/NP0.3

Satellite-based early warning system of critical transitions in forest ecosystems at living lab scale 

Deepakrishna Somasundaram, Agata Elia, Matteo Mura, Mark Pickering, and Forzieri Giovanni

Critical transition is an increasingly widespread phenomenon in global forest ecosystems, yet predicting its occurrence remains a challenge due to limited understanding of the underlying mechanisms and the variability in empirical relationships between forest health and external perturbations that can lead to critical transitions.

In this study, we demonstrate that the temporal loss of resilience, quantified in terms of critical slowing down (CSD) indicators, can serve as an early warning system (EWS) for critical transitions in forest ecosystems. CSD indicators are analyzed by integrating MODIS satellite data-derived vegetation dynamics and disturbance events from 2000–2021 at 500 m. We applied this approach to 13 living labs distributed across Europe, South America, and China, covering a wide range of environmental gradients and forest management types. Results show that CSD indicators can efficiently capture spatial and temporal variations in critical transitions in near real time. These findings highlight the potential of this EWS for improving forest critical transition predictions as well as providing practical insights for management and adaptation strategies in the context of climate change and at a spatial scale appropriate for decision makers.

How to cite: Somasundaram, D., Elia, A., Mura, M., Pickering, M., and Giovanni, F.: Satellite-based early warning system of critical transitions in forest ecosystems at living lab scale, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16943, https://doi.org/10.5194/egusphere-egu25-16943, 2025.

EGU25-17534 | ECS | Posters on site | ITS4.1/NP0.3

Assessment of a potential regime shift in global terrestrial water storage 

Casimir Fisch, Lukas Gudmundsson, Dominik L. Schumacher, and Sonia I. Seneviratne

Tipping points have been identified in several components of the Earth system, raising concerns about abrupt and potentially irreversible changes under climate change. A recent analysis of GRACE satellite data reveals a sudden and unprecedented decline in terrestrial water storage (TWS) during 2015–2016, coinciding with a major El Niño–Southern Oscillation (ENSO) event (Rodell et al. 2024). This decline suggests a recent net drying of the land and raises the hypothesis of a regime shift in the global terrestrial water system. Potential mechanisms include enhanced evapotranspiration, intensifying drought frequency and severity, and land–atmosphere feedbacks. Early warning signals, such as increased autocorrelation and variance observed prior to the decline, support this hypothesis.

To evaluate the significance and rarity of the observed transition, we develop a detection methodology and apply it to both observational estimates and climate model simulations. By analysing fully coupled pre-industrial control simulations, historical simulations, and AMIP-style experiments with prescribed sea surface temperatures, we aim to disentangle the roles of anthropogenic climate change and specific modes of climate variability (e.g., ENSO) in driving this transition. Furthermore, we explore the potential for transitions to alternative states in global TWS. Our work establishes a framework for understanding abrupt changes in TWS and their implications for the terrestrial water cycle in a warming climate.

References

Rodell, M., Barnoud, A., Robertson, F.R. et al. An Abrupt Decline in Global Terrestrial Water Storage and Its Relationship with Sea Level Change. Surv Geophys 45, 1875–1902 (2024). https://doi.org/10.1007/s10712-024-09860-w

How to cite: Fisch, C., Gudmundsson, L., Schumacher, D. L., and Seneviratne, S. I.: Assessment of a potential regime shift in global terrestrial water storage, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17534, https://doi.org/10.5194/egusphere-egu25-17534, 2025.

EGU25-17704 | Posters on site | ITS4.1/NP0.3

Socio-metabolic class conflicts in the Anthropocene 

Ilona M. Otto

The Anthropocene epoch is characterized by an excessive use of natural resources and energy that drives the environmental destruction of the planet. However, large inequalities exist among different social groups that benefit to various degrees from the use of resources and energy, as well as among those suffering from the negative impacts of environmental destruction. In this paper, we systematically analyze these differences and discuss a social stratification theory based not only on differences in terms of possessions or social status, but also on differences in how these groups can control and benefit from the planetary material cycles and energy flows or suffer the consequences of environmental degradation. Referring to consumption data, we propose six global socio-metabolic classes and show distinctive patterns in the energy use of these classes. More research is needed to reveal differences in the use of natural resources essential for maintaining the biosphere integrity, such as land, water, nitrogen, and phosphorus. Targeted policy measures that address excessive appropriation of energy and natural resources are needed, as are expansions in infrastructure and institutional change that supports the wellbeing of humankind, and especially of the most marginalized classes.

How to cite: Otto, I. M.: Socio-metabolic class conflicts in the Anthropocene, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17704, https://doi.org/10.5194/egusphere-egu25-17704, 2025.

EGU25-17856 | ECS | Orals | ITS4.1/NP0.3

Amazon precipitation response to an AMOC shutdown in a km-scale atmospheric model  

Keno Riechers, Cathy Hohenegger, Hauke Schmidt, Monika Esch, and Bjorn Stevens

The Atlantic Meridional Overturning Circulation (AMOC) is considered one of the Earth’s climate tipping elements. Concerns have been raised that global warming could increase the freshwater input into the North Atlantic at high northern latitudes and thereby abruptly interrupt the deep water formation that fuels the AMOC’s lower limb and is necessary to maintain the overturning. To assess the risks such an AMOC tipping scenario poses to societies, it is essential to understand how an AMOC collapse feeds back into the climate system as a whole. It is of particular interest whether an AMOC tipping would have a stabilizing or destabilizing effect on other climate tipping elements. In this context, we studied the impact of an AMOC shutdown on the Amazon Rainforest, which is itself thought to be at risk of undergoing a transition to a savanna state. We forced a km-scale atmosphere-only model with sea surface temperatures from a second lower-resolution coupled climate model simulation that features a collapsed AMOC state. Previous studies indicate that land-atmosphere interactions are different in such convection-resolving models compared to CMIP-type models, possibly affecting the response of precipitation to large-scale perturbations. In general, our simulation confirms the global AMOC-collapse induced precipitation and temperature anomaly patterns also seen in coupled climate model hosing experiments. Most prominently these comprise a cooling and drying of the North Atlantic region and a corresponding southward shift of the tropical rainbelt. However, upon closer examination, we find that over land the signal is attenuated, and in particular precipitation patterns over the Amazon Rainforest appear to be remarkably robust against an AMOC shutdown. This, in turn, means that a tipping of the AMOC would to a first degree neither have a stabilizing nor destabilizing effect on the Amazon Rainforest.

How to cite: Riechers, K., Hohenegger, C., Schmidt, H., Esch, M., and Stevens, B.: Amazon precipitation response to an AMOC shutdown in a km-scale atmospheric model , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17856, https://doi.org/10.5194/egusphere-egu25-17856, 2025.

EGU25-18362 | ECS | Orals | ITS4.1/NP0.3

Advancing the pathway towards natural capital based assessment for industrial and financial sectors 

Ming-Kuang Chung, Kuanhui Elaine Lin, and Wan-Ling Tseng

The relationship between nature and industry has been constantly contested for decades, regardless of the warning on the Earth as transformed by human action (Turner, B. L., et al., 1993) which address the unprecedented changes in the biosphere that have taken place over the last 300 years. Accumulation of the human impacts has also led to the degradation of the atmosphere resulting in anthropogenic warming that have brought tremendous threats to societies. While standing at the tipping point, international societies have made substantive advancement to push industrial and financial sectors taking responsibility in carbon accounting and climate risk assessment (i.e., TCFD). The relationship between climate and industry is complex, but the threat from both of them on biodiversity and natural capital (NC) loss is even devastating. In 2021, the initiative of Taskforce on Nature-related Financial Disclosures (TNFD) was launched and the TNFD Recommendations and Guidance is released in 2023. With a broader focus on the industrial and financial sector dependence and impact on the NC, TNFD contains a big range of ambiguity in developing methodology. Meanwhile, climate risk is regarded as a driving force of ecosystem change in the assessment. How to access relevant data, in suitable spatial and temporal resolution, to quantify the NC related dependency and risk becomes the most fundamental challenge before tipping elements and tipping interactions can be identified to facilitate a social and industrial transformation. 

This study collaborates with a listed high-tech company in Taiwan to assess the relationship between its value chain and NC following the LEAP approach. We have developed a high-spatial-resolution database to identify the dependencies and impacts on NC across different operational locations. Meanwhile, we conduct materiality assessments through internal questionnaires, examining the significance of different types of NC to business operations from the perspectives of Consequences rating and Likelihood rating. Finally, we aim to establish TNFD risk matrices by integrating the assessment results from spatial and materiality assessments, with the hope of helping enterprises to identify NC requiring immediate attention and action.

Overall, the integrated TNFD assessment method combining spatial and materiality analyses serve as tipping elements between enterprises and NC; it may help enterprises systematically quantify their dependencies and impacts on NC, thereby identifying operational locations and types of NC that require priority action. Meanwhile, high-resolution spatial databases can support enterprises in defining the locations, scope, and even causes of NC issues, which in turn can help identify key external stakeholders and initiate new engagements. This integrated assessment approach has the potential to address the methodological gaps in TNFD development and to provide a concrete empirical foundation for business operational transformation, helping enterprises to develop early adaptation and response strategies when facing global ecosystem changes.

How to cite: Chung, M.-K., Lin, K. E., and Tseng, W.-L.: Advancing the pathway towards natural capital based assessment for industrial and financial sectors, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18362, https://doi.org/10.5194/egusphere-egu25-18362, 2025.

EGU25-18552 | ECS | Orals | ITS4.1/NP0.3

News from TIPMIP 

Sina Loriani, Donovan Dennis, Jonathan F. Donges, and Ricarda Winkelmann

The Tipping Point Modelling Intercomparison Project (TIPMIP) is an international intercomparison project that aims to systematically advance our understanding of tipping dynamics in various Earth system components, and assess the associated uncertainties. By connecting and evaluating various models, TIPMIP will fill critical knowledge gaps in Earth system and climate modelling by improving the assessment of overall anthropogenic forcing and long-term commitments (irreversibilities). In this contribution, we report on the status of the project, highlighting recent advances including the finalisation of experimental protocols and first results. Moreover, we provide an overview on the established scientific infrastructure and next steps, inviting the tipping points modelling community for contributions.

How to cite: Loriani, S., Dennis, D., Donges, J. F., and Winkelmann, R.: News from TIPMIP, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18552, https://doi.org/10.5194/egusphere-egu25-18552, 2025.

We are transitioning towards a climate state on Earth featuring rapid changes in response to anthropogenic greenhouse gas emissions and land-use change, with severe observable and projected impacts on the occurrence of extreme weather events and increasing risk of crossing large-scale tipping points. Neither the transition nor the long-term climate state has been observed by (human-made) measurements before, making information on past climatic states increasingly more important to help anticipate future Earth System change. Paleoclimate records have enormously expanded over the past decades, and provide extremely rich information about physical, cryospheric, biological, and ecological processes on many spatial and temporal scales. Yet, it has been difficult so far to directly transform this knowledge on past processes into a more confident evaluation of future projections for the Earth system. In this contribution, I will summarise lessons learned from past climate change on our understanding of climate variability, abrupt changes and climate response to greenhouse gas changes and other forcing. For example, generalizations of classical measures such as equilibrium climate sensitivity can be useful in the palaeoclimate and future context for understanding the response of a climate state to radiative forcing beyond the linear regime, i.e. when (part of) the climate system is close to a tipping point. Finally, this contribution will present the ambition and programme of the starting EU-HORIZON project Past-to-Future (P2F) aiming at developing, expanding and using the wealth of paleoclimate data to improve existing Earth System Models in terms of their ability to describe possibly exotic, out of sample, climate states and the transition pathways towards them from current conditions.

How to cite: von der Heydt, A.: Past to future: Towards fully paleo-informed future climate projections, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19085, https://doi.org/10.5194/egusphere-egu25-19085, 2025.

EGU25-19501 | Posters on site | ITS4.1/NP0.3

ISOTIPIC: Greenland ice sheet potential for tipping with the Earth System Model UKESM-ice 

Charlotte Lang, Robin Smith, Steve George, Robert Marsh, and Bablu Sinha

As part of a project exploring the relation between the Greenland ice sheet stability and the AMOC, we present coupled climate and ice sheet simulations of Greenland with the Earth System Model (ESM) UKESM, a state-of-the-art ESM capable of representing the interactions between ice sheets and the atmosphere and their co-evolution (UKESM-ice; Smith et al., 2021).
Recent large ensemble exercises indicate that there is no sign of non-linear volume change or irreversibility at the scale of the Greenland ice sheet in UKESM-ice, even at high warming levels and despite large ice losses.
We present new simulations exploring Greenland's potential for tipping with modified (snow and ice sheet) parameters and including a recently developed scheme for the marine forcing of outlet glaciers, which was previously omitted from UKESM-ice and prevented the representation of the direct influence of the ocean on the Greenland ice sheet. Results show linear trends of (large) ice volume change at the scale of the ice sheet but local evidence of accelerating melt along the South West margin.
Next steps in the project include providing fresh water from UKESM-ice surface runoff and solid discharge of icebergs to investigate their effect on the strength of the AMOC in NEMO simulations and using a new high resolution NEMO dataset as ocean forcing of the ice sheet in UKESM-ice. 

How to cite: Lang, C., Smith, R., George, S., Marsh, R., and Sinha, B.: ISOTIPIC: Greenland ice sheet potential for tipping with the Earth System Model UKESM-ice, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19501, https://doi.org/10.5194/egusphere-egu25-19501, 2025.

EGU25-19773 | Orals | ITS4.1/NP0.3

 Navigating multiscale social tipping dynamics to stabilise Earth’s climate 

Andrew Ringsmuth, Andrew Tilman, Jordan Everall, Emanuele Campiglio, Magdalena Pieler, Sara Constantino, and Ilona Otto

Mounting evidence that human activities are driving Earth’s climate toward dangerous tipping points has raised the question of whether these may be averted by quickly reaching tipping points in human societies. Prior work on social tipping dynamics has focused mainly on defining its key features, identifying and characterising important social tipping elements, and operationalizing interventions for triggering individual elements. However, the success of climate-stabilizing interventions will depend on their timing and coordination across multiple tipping elements that operate on different characteristic time scales, and these coupled dynamics are currently not understood. In this work we explore the challenges of intervention timing and the potential to coordinate subsystem tipping cascades in a multiscale system to achieve a timely whole-system transition. We develop a stylized model in which the changing climate is coupled to a network of social tipping elements such as public support for climate action, political policymaking, financial investment in energy technologies, and energy infrastructure substitution, each with its characteristic dynamics and time scales. We study how intervention timing interacts with tipping cascades between subsystems and derive principles for navigating the system to the desired state. Additionally, we analyze the effects of `windows of opportunity’ - unpredictable system shocks that are likely to become more frequent as climate change intensifies - on our model transformation pathways, and ascertain how these may be exploited to disrupt system-stabilizing feedbacks and synchronize subsystem changes. Our findings emphasise the importance of a complexity-based understanding of human agency and governance of the world-Earth system.

How to cite: Ringsmuth, A., Tilman, A., Everall, J., Campiglio, E., Pieler, M., Constantino, S., and Otto, I.:  Navigating multiscale social tipping dynamics to stabilise Earth’s climate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19773, https://doi.org/10.5194/egusphere-egu25-19773, 2025.

EGU25-19783 | ECS | Orals | ITS4.1/NP0.3

Global stability of the AMOC under CO2 forcing: Boundary crisis, long transients and oscillatory edge states 

Reyk Börner, Oliver Mehling, Jost von Hardenberg, and Valerio Lucarini

There is growing concern that the Atlantic Meridional Overturning Circulation (AMOC), a vital Earth system component, could weaken or even collapse under climate change. Despite the severe potential impacts associated with such a transition, it remains extremely challenging to reliably estimate the proximity to a critical threshold and to predict the AMOC's fate under future anthropogenic forcing. We argue that a global viewpoint on the dynamics beyond the detection of early-warning signals is needed for a robust risk assessment. Here we explore the phase space of an intermediate-complexity earth system model, PlaSim-LSG, featuring a multistable AMOC. For two different atmospheric carbon dioxide (CO2) levels, we explicitly compute the Melancholia (M) state that separates the strong and weak AMOC attractors found in the model. The M state is a chaotic saddle embedded in the basin boundary between the competing states (an edge state). We show that, while being unstable, the M state can govern the transient climate for centuries. The M state exhibits strong AMOC oscillations on centennial timescales driven by sea ice and oceanic convection in the North Atlantic. Combining these insights with simulations under future CO2 forcing scenarios (SSPs), we demonstrate that in our model the AMOC undergoes a boundary crisis at CO2 levels projected to be reached in the next decade. Near the crisis, the AMOC behavior becomes highly unpredictable. Founded in dynamical systems theory, our results offer an interpretation of the so-called stochastic bifurcation recently observed in a CMIP6 earth system model under the same time-dependent forcing scenario.

How to cite: Börner, R., Mehling, O., von Hardenberg, J., and Lucarini, V.: Global stability of the AMOC under CO2 forcing: Boundary crisis, long transients and oscillatory edge states, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19783, https://doi.org/10.5194/egusphere-egu25-19783, 2025.

EGU25-20396 | ECS | Posters on site | ITS4.1/NP0.3

Dynamics-informed deep learning for tipping point forecasting 

Carla Roesch and Christina Last

As the world enters a period of accelerated climate change, we require the rapid development of an early warning system (EWS) that identifies whether climatic conditions will result in reaching a tipping point. Tipping points represent critical thresholds where a small disturbance can cause a significant, qualitative shift in a system's state that can have crucial effects on human livelihoods. The impacts of political developments on future emission pathways, highlights the need for warning systems focused on climate risk communication that can be deployed and updated easily by policy teams with data pertaining to representative emission profiles. We are developing an early warning system to detect tipping points using a combination of observational and model data. In this abstract, we introduce the Tipsy-API platform; a dynamics-informed deep learning model to forecast relevant thresholds of the Greenland ice sheet and Atlantic Meridional Ocean Circulation. Following the objective of a “real time” warning system, our framework  iteratively updates forecasts with new observations to adjust the tipping point prediction accordingly. Finally, the framework will be deployed online and be available as an API, which we aim to be interactive and iteratively updated once new information about future warming becomes available. This ongoing work attempts to understand and address the requirements of a UK Government R&D funding agency, with the remit of engaging in high risk and high reward climate research. Thus, our project aims to both reduce uncertainty about tipping points and to allow for necessary open communication with policy makers and other relevant stakeholders.

How to cite: Roesch, C. and Last, C.: Dynamics-informed deep learning for tipping point forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20396, https://doi.org/10.5194/egusphere-egu25-20396, 2025.

EGU25-21133 | Orals | ITS4.1/NP0.3

Slowing Down of the Atlantic Meridional Overturning Circulation Due to Excess Freshwater: Insights from Turbulence-Resolving Simulations 

Bahman Ghasemi, Bishakhdatta Gayen, Catherine Vreugdenhil, and Taimoor Sohail
The Atlantic Meridional Overturning Circulation (AMOC) plays a crucial role in the global climate system by transporting heat, salt, and nutrients across ocean basins. Its stability hinges on the complex interplay between temperature and salinity, although the precise contributions of these factors remain unclear. This highlights the need for systematic investigations to better understand and predict AMOC behavior in a changing climate. In this study, we use turbulence-resolving simulations with a laboratory-scale model of the North Atlantic Ocean to examine how thermal, salinity, and wind forcing influence large-scale ocean circulation. By varying the relative impacts of salinity and temperature forcing, we find that increasing salinity forcing slows the AMOC by weakening deep convection and shifting the subtropical gyre southward. This slowdown reduces northward heat and salt transport, leading to warming and salinification in the northern subtropics and cooling in subpolar regions. Salt-finger convection further amplifies subtropical warming and salinification. On the other hand, a sufficiently strong thermal forcing in a weakened AMOC state can trigger a significant rebound in AMOC strength. Wind stress was also found to enhance both the AMOC and gyre strength. Future climate projections indicate that freshwater forcing will become increasingly significant, and our results suggest that greater salinity forcing will further slow the AMOC and reduce meridional tracer transport. These findings are essential for improving large-scale ocean models and advancing our understanding of temperature-salinity feedback mechanisms in global ocean circulation.

 

How to cite: Ghasemi, B., Gayen, B., Vreugdenhil, C., and Sohail, T.: Slowing Down of the Atlantic Meridional Overturning Circulation Due to Excess Freshwater: Insights from Turbulence-Resolving Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21133, https://doi.org/10.5194/egusphere-egu25-21133, 2025.

In China's drylands, deserts and areas prone to desertification constitute 44% of the landscape. The desert-oasis transition zone serves as a critical buffer between the desert interior and the oasis, playing an essential role in managing and preventing desertification. Despite its importance, the question of whether ecosystem functions exhibit multistability and experience regime shifts from functional to desertified states remains unresolved, particularly concerning the relationship between changes in vegetation patterns and ecosystem state transitions at the desert edges of arid and hyper-arid regions. In this study, we examined the stability landscapes of ecosystem multifunctionality and vegetation patterns in response to decreasing precipitation at both the inter-desert scale and within individual deserts, as the distance from the oasis to the desert interior increases. We compared the precipitation and distance thresholds for abrupt changes in vegetation pattern indices with those for regime shifts in ecosystem multifunctionality. Our analysis revealed that ecosystem multifunctionality can exist in both functional and desertified states when precipitation ranges between 104.37 mm and 152.56 mm. However, when precipitation drops below 104.37 mm, a complete shift from a functional to a desertified state occurs. The average precipitation threshold for abrupt changes in vegetation pattern indices—such as the size, shape complexity, and connectivity of vegetation patches, flow length, spatial skewness of the landscape, and the power law range, cutoff, and plexpo of the vegetation patch size distribution—is 201.69 ± 34.87 mm, which is higher than the threshold for ecosystem multifunctionality regime shifts. At the scale of individual deserts, changes in vegetation patterns precede regime shifts in ecosystem multifunctionality. These findings suggest that vegetation pattern indices can serve as early warning indicators for desertification in extremely arid desert-oasis transition zones. This study contributes to the enhancement of early-warning systems and supports the monitoring of desertification processes.

How to cite: Li, C. and Zhou, W.: Vegetation patterns as early warning signals for shifts in ecosystem multifunctionality in the desert-oasis transition zone of China’s drylands , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1786, https://doi.org/10.5194/egusphere-egu25-1786, 2025.

Abstract: Climate models often predict that more extreme precipitation events will occur in arid and semiarid regions, where plant phenology is particularly sensitive to precipitation changes. To understand how increases in precipitation affect plant phenology, this study conducted a manipulative field experiment in a desert ecosystem of northwest China. In this study, a long-term in situ water addition experiment was conducted in a temperate desert in northwestern China. The following five treatments were used: natural rain plus an additional 0, 25, 50, 75, and 100% of the local mean annual precipitation. A series of phenological events, including leaf unfolding, fruit setting (onset, summit and end), fruit ripening (onset, summit and end) and leaf coloration of the locally dominant shrub Nitraria tangutorum were observed from 2012 to 2018. The results showed that on average, over the seven-year-study and in all treatments water addition treatments advanced the leaf unfolding date by 1.29–3.00 days, but delayed the leaf coloration date by 1.18–11.82 days. Therefore, the length of the growing season was prolonged by 2.11–13.68 days. However, water addition treatments had no significant effects on all six fruiting events in almost all years, and the occurrence time of almost all fruiting events remained relatively stable compared with leaf phenology. The inter-annual variations of fruiting events were driven by the preceding flowering events rather than temperature or precipitation.

How to cite: Bao, F.: Contrasting responses of fruiting phenology and folia phenology to water additiontreatments in the Desert Shrub Nitraria tangutorum, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2220, https://doi.org/10.5194/egusphere-egu25-2220, 2025.

EGU25-3466 | ECS | Posters on site | ITS4.20/NP0.4

Exploring the impacts of active faulting & tectonics on the vegetation cover of the dynamic Serengeti-Mara and Ngorongoro ecosystems of East Africa through spectral index analysis 

Chintan Purohit, Alina Ludat, Alfred Said, Revocatus Machunda, Tobias Hank, Beth Kahle, and Simon Kuebler

The study of how topographic and geological complexities drive vegetation dynamics over extended timescales, provides critical insights into the interactions between landscapes and ecosystems. Our study area encompasses the Greater Serengeti-Mara Ecosystem (GSME) in the Kenya-Tanzania transboundary region, renowned for its ecological richness and dynamic environments, most famously as the setting for the world’s largest terrestrial mammal migration. We focus on two case study regions: the Mara River Basin (MRB) and the Ngorongoro Conservation Area (NCA) to investigate localized interactions between geological, topographic, and ecological processes. The ecosystems are supported by a healthy and diverse vegetation cover, impacted by natural as well as anthropogenic factors. MRB is bounded in the north by active normal faulting dominated by Utimbara and Isuria faults whereas NCA is centred on Ngorongoro Crater, a large volcanic caldera. The tectonics of NCA is well-studied but subrecent faulting of Utimbara and Isuria was previously unrecognised and the impacts of these faults on uplift, subsidence and tilting of MRB has been revealed only recently. Previous studies have explored the relationship between precipitation and vegetation dynamics in the region. Limited research has focused on soil properties, primarily examining the effects of volcanic ash on the southeastern sector of GSME. However, the role of tectonics in influencing vegetation and, by extension, the broader ecosystem remains underexplored. We used remote sensing data (Landsat 5, 7, 8 and Sentinel 2) to create a time series analysis from the years 1984 until 2024 to examine the changes in the vegetation cover in the study area. Landsat 7 & 8 and Sentinel 2 data were processed in Google Earth Engine whereas those from Landsat 5 & 7 using Erdas Imagine. The normalised differential vegetation index (NDVI) shows a clear difference in vegetation cover during wet and dry seasons throughout the four decades for both the regions. MRB, which is covered by Quaternary sediments, has a higher vegetation cover throughout the year. NCA is affected by intermittent ash eruptions from Oldoinyo Lengai and has a vegetation cover, which varies at differing altitudes within the region and also shows a considerable seasonal variation at lower altitudes. Additionally, there is a significant difference in precipitation between MRB and NCA. In such a scenario, the vegetation cover in both the regions is likely to be a function of the interaction between the inherent soil properties and precipitation. Interestingly, stable vegetation also persists along active faults. Fault escarpments and fault-bounded wetlands provide seasonally stable vegetation cover, potentially due to localized influences on hydrology and soil properties and may serve as refugia during dry seasons. Our preliminary results highlight the need to integrate geo-tectonic analysis into broader ecosystem studies to better understand their role in sustaining biodiversity and ecosystem resilience.

How to cite: Purohit, C., Ludat, A., Said, A., Machunda, R., Hank, T., Kahle, B., and Kuebler, S.: Exploring the impacts of active faulting & tectonics on the vegetation cover of the dynamic Serengeti-Mara and Ngorongoro ecosystems of East Africa through spectral index analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3466, https://doi.org/10.5194/egusphere-egu25-3466, 2025.

EGU25-3816 | Orals | ITS4.20/NP0.4

The origin of the elongated fairy circles in the Giribes Plains, northwest Namibia 

Hezi Yizhaq, Stephan Getzin, Itzhak katra, Nina Kamennaya, Yehuda Peled, and Ehud Meron

 

Fairy circles are exceedingly regularly spaced barren circular patches in arid landscapes, typically encircled by a ring of taller grasses. These vegetation patterns occur in Southwestern Africa and Australia and have also been suggested to occur in North Africa, Middle East and Madagascar. The enigmatic origins of fairy circles in arid landscape shave intrigued ecologists and sparked heated debate about the two main competing hypotheses: the termite origin and vegetation self-organization hypotheses.

In the southern part of the Giribes Plains, Kunene region, northwest Namibia, fairy circles form in a distinctive, chain-like arrangement along drainage lines that run from north to south, closely aligned along a slope. These fairy circles are unusual in their extreme elongation, with the most extreme case measuring 32.5 meters long and only 7.7 meters wide. In contrast, the fairy circles in the rest of the Giribes outside the drainage lines are typically circular and exhibit a highly ordered, hexagonal pattern. Based on field work, remote sensing and mathematical modeling we explain the formation of these unique fairy circles.

The soil in the matrix between the circles is covered by physical crust, with some areas featuring a thin biocrust. This is the only place in Namibia where soil crust developed in the matrix. This crust causes the matrix soil to be nearly four times more compact than the soil within the fairy circles. The sand within the fairy circles is coarser (D50 ~600 µm) compared to the matrix soil (D50 ~300 µm), which supports the formation of the crust. Interestingly, sand in fairy circles not aligned with the drainage lines is also coarser (D50 ~450 µm). Hydraulic conductivity, measured using a mini-disk infiltrometer, is three to four times greater within the fairy circles than in the surrounded matrix.

Building on these field observations, we hypothesize that the elongated shape of the fairy circles results from anisotropic soil water diffusion. Water diffuses more readily along the drainage lines than in the surrounding matrix, causing the fairy circles to expand more rapidly along the watercourses than laterally. To test this hypothesis, we used the mathematical model of Zelnik et al. (2015), which simulates biomass and soil water densities under varying water-soil diffusion coefficient ratios, r (r=1outside the drainage lines and r>1 inside the fairy circle) and precipitation rates .

The simulations indicate that, for moderate diffusion ratios and varying precipitation rates, elongated fairy circles form along the drainage lines, while circular fairy circles emerge when the diffusion ratio is lower. The results agree with remote sensing analysis of images take from a drone.  The stability of the pattern to different precipitation rates and r values was also studied. These results support the hypothesis that anisotropic soil water diffusion contributes to the elongated shape of the fairy circles in the Girbies plain, although other factors may also play a role. Indirectly our work supports the self-organization hypothesis for the origin of fairy circles.  The formation of the crust in the matrix remains is still an open question for future research.

 

How to cite: Yizhaq, H., Getzin, S., katra, I., Kamennaya, N., Peled, Y., and Meron, E.: The origin of the elongated fairy circles in the Giribes Plains, northwest Namibia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3816, https://doi.org/10.5194/egusphere-egu25-3816, 2025.

Dryland aeolian landscapes are among the most vulnerable ecosystems under accelerating climate shift and land-use changes, where complex interactions between vegetation, soils, and landforms play a crucial role in maintaining ecosystem resilience and services. This study integrates remote sensing, field surveys, and numerical modeling to explore the coevolution of vegetation and aeolian landforms over the past four decades in East Asia’s arid regions, with a particular focus on the feedback mechanisms driving landscape stability in the arid zones under climatic and human forcing.
Analyses of aeolian landforms and climate systems in northern China reveal that declining wind speeds, associated with global terrestrial stilling, have significantly slowed dune migration rates over the past few decades, while widespread vegetation recovery has stabilized dune fields and mitigated desertification. Restoration practices, such as straw checkerboards, have accelerated vegetation recovery, increasing biodiversity and stabilizing soils, though soil fertility remains low compared to natural systems. Dust activity, an integral component of aeolian systems, have been suppressed in these areas, largely due to both climatic shifts and these large-scale restoration projects. Finally, high-resolution satellite images and field observations highlight how vegetation expansion modifies dune morphology through processes such as vegetation anchoring and sand transport alteration, leading to transitions from active to stabilized states. Conceptual models of vegetated dune morphodynamics provide insights into the role of vegetation-soil-landform feedbacks in shaping the arid landscapes.
This study emphasizes the interconnectedness of climate systems, vegetation dynamics, soil properties, and aeolian processes in maintaining ecosystem resilience and restoring ecosystem services. By linking dune morphologies and vegetation dynamics to thresholds of stability and nonlinear responses to climatic and anthropogenic pressures, the findings contribute to a deeper understanding of how dryland ecosystems adapt and evolve. These insights support more effective strategies for soil conservation, landform stabilization, and the restoration of ecosystem functions in the face of ongoing climate and land-use changes.

How to cite: Xu, Z., Wang, L., and Pang, X.: Deciphering Aeolian Landscape Dynamics: Vegetation Recovery and Dune Stabilization under Climatic and Human Influences, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4912, https://doi.org/10.5194/egusphere-egu25-4912, 2025.

EGU25-5142 | Posters on site | ITS4.20/NP0.4

Accounting for Vegetation Feedbacks in Hydrological Models Using a New Vegetation-aware Evapotranspiration Formulation 

Carlos Brieva, Eliana Jorquera, Juan Quijano, George Kuczera, Patricia Saco, Jose Rodriguez, and Golam Kibria

Streamflow in several catchments in eastern Australia has decreased considerably (up to 40%) over the past 20 to 30 years, despite stable rainfall levels. This decoupling of streamflow and rainfall undermines the predictive accuracy of rainfall-runoff models used by catchment managers, which typically rely on the assumption of a stable relationship between these variables. Similar non-stationarity in streamflow has been observed in other catchments in the world, and evidence suggests that vegetation processes may be driving this non-stationarity due to increases in temperature and CO2. Current rainfall-runoff models fail to capture the impact of these vegetation changes on evapotranspiration (ET). While these models account for ET's dependence on soil moisture, they do not consider changes in vegetation biomass and health, which can significantly alter ET and, consequently, runoff.

This contribution presents a methodology for estimating a vegetation-aware ET based on the Penman-Monteith equation and emulators that can account for changes in vegetation biomass and health. The emulators are developed using data from the Australian and New Zealand Flux Research and Monitoring network (TERN OzFlux). This network provides extensive measurements of energy, carbon, and water exchanges across various ecosystems, from which vegetation effects can be estimated under different environmental conditions, and across different vegetation types. Through this research we aim to contribute to understanding evapotranspiration dynamics and offer a reliable and simple tool for estimating vegetation effects, ultimately adding it to more realistic rainfall-runoff simulations.

How to cite: Brieva, C., Jorquera, E., Quijano, J., Kuczera, G., Saco, P., Rodriguez, J., and Kibria, G.: Accounting for Vegetation Feedbacks in Hydrological Models Using a New Vegetation-aware Evapotranspiration Formulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5142, https://doi.org/10.5194/egusphere-egu25-5142, 2025.

Salt-tolerant Tamarix chinensis roots are crucial in preserving wetland soil and carbon  sequestration, which is essential for wetland ecology. Soil-water-salt conditions influence the growth of these roots in coastal saline areas, but the specific factors and their effects remain unclear. Using principal component and partial least square structural equation modelling (SEM) methods, we studied T. chinensis root features in six Yellow River delta communities. Results showed varied root features across locations, with larger roots further inland. Root growth negatively correlated with soil texture and salinity and positively with groundwater levels. Soil texture and salinity decreased with distance from the coast, while groundwater increased with distance from the Yellow River. This suggests that geographical location influences soil water-salt conditions, impacting root characteristics. The principal component analysis–derived root feature index captured 56.7% of root feature variation. SEM revealed geographical locations indirectly influence root features, with the Yellow River’s proximity primarily affecting them through groundwater and coastal distance influencing via soil sand content and salinity. The study underscores the importance of these findings for wetland conservation and ecology.

How to cite: lizhu, S.: Soil spatial heterogeneity created by river–sea interaction influences Tamarix chinensis root features in the Yellow River Delta, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5353, https://doi.org/10.5194/egusphere-egu25-5353, 2025.

EGU25-5452 | ECS | Posters on site | ITS4.20/NP0.4

Mapping Shrub Fractional Abundance: A Multi-Scale Remote Sensing and Machine Learning Framework for Arid Ecosystem Monitoring 

Zhonghua Liu, Xin Cao, Josep Peñuelas, Adrià Descals, Dedi Yang, Lingli Liu, Yanjun Su, Liangyun Liu, Jin Chen, and Jin Wu

Shrubs, characterized by their multiple dwarf stems, are a dominant plant functional type in arid and semi-arid regions, which cover 40% of Earth's land surface. These ecosystems are fragile and highly susceptible to climate change and human disturbances. The abundance of shrubs serves as an important indicator of ecosystem health, and their projected increase due to CO₂ fertilization and warming climates could significantly alter ecosystem functioning, exacerbate desertification, and impact essential ecosystem services. Monitoring shrub fractional abundance—the proportion of vegetative cover occupied by shrubs—is crucial for understanding these dynamics and guiding sustainable management practices. However, mapping shrub fractional abundance over large areas presents challenges due to their small crowns, sparse distribution, and high density, rendering traditional field surveys and conventional satellite remote sensing techniques inadequate. In this study, we propose an innovative two-step approach that integrates sub-meter resolution Google Earth (GE) imagery with decametric-resolution Sentinel-2 time-series data for accurate and scalable shrub fractional mapping. Our methodology consists of two main steps: (1) a semi-automatic process that uses GE imagery to delineate 1.31 million shrub crowns and generate high-quality training data, and (2) a machine learning model that combines spectral and phenological features from Sentinel-2 data to upscale GE-derived shrub fractional abundance across diverse arid and semi-arid landscapes in Inner Mongolia, China. The model achieved strong predictive accuracy (= 0.70), with phenological features—particularly during early May, mid-June, and late September—proving critical for distinguishing shrubs from seasonal vegetation. These periods correspond to key phenophases, including germination, peak growth, and senescence of grasses, which contrast with the perennial phenology of shrubs, highlighting the significance of phenology in differentiating shrubs from dynamic seasonal vegetation. Our results demonstrate the effectiveness of integrating multi-scale remote sensing data with machine learning to address existing limitations in shrub monitoring. This approach provides a scalable and transferable framework for global mapping of shrub fractional abundance, offering valuable insights into shrub encroachment and its implications for ecosystem health in the context of changing climatic and anthropogenic conditions.

How to cite: Liu, Z., Cao, X., Peñuelas, J., Descals, A., Yang, D., Liu, L., Su, Y., Liu, L., Chen, J., and Wu, J.: Mapping Shrub Fractional Abundance: A Multi-Scale Remote Sensing and Machine Learning Framework for Arid Ecosystem Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5452, https://doi.org/10.5194/egusphere-egu25-5452, 2025.

Badlands are characterized by highly eroded, rugged landscapes with steep slopes, limited vegetation, and significant soil degradation. In badlands, vegetation plays a key role in erosion mitigation by intercepting runoff and acting as a significant factor in soil stability. However, vegetation dynamics in such an environment are determined by geomorphological factors like slope, erosion, sediment flux, and climatic conditions, characterized by temperature and precipitation patterns.

This study evaluates the significance of such drivers of vegetation transition within the badland systems using a State-and-Transition Model (STM) approach. This model predicts vegetation dynamics as a function of two basic processes: extinction (loss of vegetation) and colonization (vegetation growth over a barren patch of land). It is forced with vegetation states at four different time points (i.e., 1982, 1994, 2015, and 2021), while climate variables (e.g., temperature and precipitation), and sediment fluxes are averaged for the periods between these states. Geomorphological parameters (i.e., topographic elevation and slope) are assumed to be constant throughout the simulation period. It estimates vegetation transition probabilities using logistic regression. The model parameters are optimized through Bayesian methods (i.e., Markov Chain Monte Carlo algorithm) for climate conditions and geomorphology in the Laval catchment in the Draix-Bléone critical zone observatory, southeastern France. Model performance is quantified through repetitive training and testing to ensure the soundness of the predictions.

The results indicate that colonization is negatively impacted by higher slopes and annual sediment fluxes and is supported by increasing mean annual temperatures and summer precipitation. In contrast, vegetation extinction is driven mainly by geomorphic disturbances (e.g., slope and sediment fluxes during extreme events), while climatic factors seem to have little impact on vegetation extinction in this study area. Indeed, the forward prediction model, initiated using the 1982 vegetation state with best-fit parameters as forcing, resulted in a reasonably close match of the predicted states to the conditions observed, i.e., those of 1994, 2015, and 2021, which had an accuracy of ~0.8, with uncertainties of around ~0.35.

The present study integrates both geomorphological and climatic data to develop valid interpretations concerning environmental factors responsible for vegetation dynamics within badland topography, adding to an improved understanding of the ecosystem dynamics of these sensitive environments.

How to cite: Sharma, H., Le Bouteiller, C., and Boulangeat, I.: Geomorphic and climate-driven vegetation dynamics in badlands – A case study from Laval catchment, Draix-Bléone critical zone observatory, SE France, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6012, https://doi.org/10.5194/egusphere-egu25-6012, 2025.

EGU25-7446 | ECS | Orals | ITS4.20/NP0.4

Impact of Roads on Vegetation Dynamics in the Semi-Arid Baringo County, Kenya 

Nicodemus Nyamari, Sophie Nitschke, Tanja Kramm, Dennis Otieno Ochuodho, Georg Bareth, and Christina Bogner

The semi-arid lowlands of Baringo County, Kenya provide numerous ecosystem services to pastoral and agro-pastoral communities. However, these services have been significantly impacted by gradual changes in land cover, climate change, shrub encroachment, and invasion of grasslands by species like Prosopis juliflora. This study aimed to investigate how changes in land cover and roads affect vegetation dynamics between 2000 and 2024. This period was chosen due to the availability of consistent satellite-derived Normalized Difference Vegetation Index (NDVI) data for time series analysis. Using the Complete Ensemble Empirical Mode Decomposition with Adaptive Noise (CEEMDAN), we analyzed NDVI data for five land cover classes, namely: natural shrubland, artificial grassland, forest, irrigated land, and Prosopis-infested areas. The impact of roads was assessed by calculating the instantaneous energy of high-frequency Intrinsic Mode Functions (IMFs) at buffer distances of 100, 250, 500, 1000, and 1500 meters from the roads in natural ecosystems. The results revealed diverse NDVI trends for different land cover classes. Forest exhibited mixed trends, with some pixels showing positive trends while others remained stable over time. Irrigated agricultural land indicated an increase in trend until 2017, after which it plateaued. Shrubland and artificial grassland maintained steady NDVI values with modest positive trends. Prosopis-infested areas exhibited a positive trend from 2000 to 2017, followed by a decline, likely linked to community-led invasion management efforts. The positive NDVI trends observed in forests and natural shrublands may be attributed to an increased invasion of Prosopis. Seasonal variations were associated with climatic conditions. Statistical analysis indicated that distance from the road had a significant difference on instantaneous energy but with a small effect size. These findings contribute to understanding how infrastructure and land use changes influence vegetation, providing valuable insights for sustainable management of semi-arid rural landscapes.

How to cite: Nyamari, N., Nitschke, S., Kramm, T., Otieno Ochuodho, D., Bareth, G., and Bogner, C.: Impact of Roads on Vegetation Dynamics in the Semi-Arid Baringo County, Kenya, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7446, https://doi.org/10.5194/egusphere-egu25-7446, 2025.

EGU25-7458 | Posters on site | ITS4.20/NP0.4

Effects of climate and human activities on mangrove wetland evolution. 

Eliana Jorquera, Jose Rodriguez, Patricia Saco, Steven Sandi, Juan Quijano, and Angelo Breda

Mangrove wetlands are one of the most significant and vulnerable ecosystems in the world, providing a wide range of services including habitat, flood control and carbon storage, among others. Their vulnerability under climate change scenarios has been well documented, but recent works have shown that coastal wetlands have the capacity to accrete following the trend of SLR under particular circumstances. Suspended sediment concentration (SSC) plays a critical role in the accretion mechanisms that support wetland survival.

Wetlands in the Pacific Islands are among the most vulnerable areas to climate change and they receive considerable sediment from croplands (sugarcane) of their inland catchments. This contribution focuses on mangrove wetlands at the mouth of rivers draining into the Great Sea Reef. The objectives of our research are to evaluate the sediment loads from the catchment upstream of the coastal wetlands and to model the ecogeomorphological feedbacks among catchment, wetland and coastal reef lagoon under current conditions and future climate change scenarios. The methodology simulates the hydro-sedimentological behaviour of the watershed, under current and future scenarios with changes in land use (cropland expansion/management) and extreme events (cyclones). The output of this simulation constutute the input for the eco-geomorphological coastal wetland modelling.

This integrated modelling approach provides a better understanding of the main processes and feedbacks among vegetation, sediments and hydrodynamics within the coastal wetland, considering its interactions with the adjacent terrestrial (catchment) and aquatic (reef lagoon) ecosystems.

How to cite: Jorquera, E., Rodriguez, J., Saco, P., Sandi, S., Quijano, J., and Breda, A.: Effects of climate and human activities on mangrove wetland evolution., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7458, https://doi.org/10.5194/egusphere-egu25-7458, 2025.

EGU25-9937 | ECS | Posters on site | ITS4.20/NP0.4

Efficient and realistic modelling of individual runoff events in ecohydrological systems  

Karl Kästner and Christoph Hinz

The different temporal scales of surface flow and vegetation growth represent a major challenge when simulating the dynamics of ecohydrological systems. The much faster surface flow is therefore commonly simplified by treating it as stationary and linearizing the equations. While the simplified equations can be solved efficiently, they do not resolve individual runoff events. However, the sequence of events can be relevant for the dynamics of dryland vegetation. The nonlinear flow during individual precipitation events can be resolved by employing more sophisticated numerical methods, such as adaptive-time stepping and implicit time-integration. However, this requires the iterative solution of a sequence of discrete linear systems at each time step. This is complicated by asymmetry of the discrete system, originating from the advection of the flow. Here, we explore strategies for the efficient simulation of the nonlinear flow during individual precipitation events when modelling vegetation dynamics over centuries.

How to cite: Kästner, K. and Hinz, C.: Efficient and realistic modelling of individual runoff events in ecohydrological systems , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9937, https://doi.org/10.5194/egusphere-egu25-9937, 2025.

EGU25-11850 | ECS | Posters on site | ITS4.20/NP0.4

Vegetation patterning dynamics induced by non-local connections 

Sara Filippini, Jost von Hardenberg, and Luca Ridolfi

Spatial self-organization is a common response of arid and semi-arid ecosystems to water stress. It may result in periodic patterns such as dots, gaps and labyrinths, or in more irregular arrangements such as scale-free patterns, characterised by a power law distribution of patch sizes. As pattern formation occurs over large spatial domains, in the order of km2 , it is often subject to heterogeneous environmental and soil conditions, which may lead to the anisotropic diffusion of resources.

In our project, we study the effects of anisotropic diffusion on pattern formation through the modelling of vegetation dynamics on complex network topologies. 

 

We employ the well-known reaction-diffusion vegetation model by Gilad et al. [1], in its simplified two-equation version by Zelnik et al. [2]. Two partial differential equations describe the dynamics of soil water and biomass densities.

In our implementation, the diffusive terms refer to network Laplacia, which allows us to the modify the topology on which the model operates.

When the diffusion networks of both water and biomass are regular two-dimensional lattices, we reproduce the observed progression of periodic patterns from gaps to labyrinths to dots for decreasing precipitation. 

To increase the complexity and connectivity of the network we implement the Watts-Strogatz small-world network model [3], in which a controlled number of random shortcuts is drawn over the two-dimensional lattice. Thus the number of shortcuts in the water and biomass diffusion networks become model parameters which may be used as proxies of heterogenous conditions affecting the diffusion of water and biomass respectively.

 

Our preliminary results show that an increase in anisotropic diffusion (number of shortcuts) has similar effects to an increase in isotropic diffusion in regards to the global variables of the ecosystem, such as average water and biomass densities. However, a small-world network topology induces the formation of steady-state non-periodic patterns, included scale free patterns, in a certain interval of network connectedness. 

Further, these steady-state scale free patterns appear unstable to the expansion of the largest gaps, leading to rapid desertification following a disturbance that may originate from grazing or human intervention. Hence, we uncover the existance of a bistability between two non-periodic patterns with very different ecological value. 

 

[1] E. Gilad, J. von Hardenberg, A. Provenzale, M. Shachak, and E. Meron. Ecosystem Engineers: From Pattern Formation to Habitat Creation. Physical Review Letters, 93(9):098105, 2004.

[2] Y. R. Zelnik, E. Meron, and G. Bel. Gradual regime shifts in fairy circles. Proceedings of the National Academy of Sciences, 112(40):12327–12331, 2015. 

[3] M. E. J. Newman and D. J. Watts. Scaling and percolation in the small-world network model. Physical Review E, 60(6):7332–7342, 1999.

 

How to cite: Filippini, S., von Hardenberg, J., and Ridolfi, L.: Vegetation patterning dynamics induced by non-local connections, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11850, https://doi.org/10.5194/egusphere-egu25-11850, 2025.

Dryland vegetation forms spatial patterns as an adaptation to water stress, driven by the uneven distribution of resources. While these patterns aid plant survival, herbivore grazing adds pressure, increasing desertification risks through vegetation loss and soil erosion. We present a novel model integrating vegetation patterning and herbivore grazing dynamics to explore their feedback loops over time. The model accounts for herbivore behaviors, including foraging, movement, and vegetation preferences. Using numerical continuation methods, we analyze solutions such as uniform and patterned vegetation-herbivore dynamics. A key finding is the emergence of traveling waves, where vegetation and herbivores propagate across the landscape. Herbivore distribution within these waves is asymmetric, causing uneven grazing stress. Surprisingly, this dynamic reduces overall grazing impact, enhancing vegetation sustainability compared to uniform grazing. Understanding these dynamics is vital for food security in drylands. By balancing herbivore populations and preserving vegetation, these interactions help mitigate drought and population growth challenges.

How to cite: Singha, J.: Traveling vegetation-herbivore waves can sustain ecosystems threatened by droughts and population growth, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19596, https://doi.org/10.5194/egusphere-egu25-19596, 2025.

EGU25-19726 | Orals | ITS4.20/NP0.4

Towards Standardising Runoff Connectivity Assessment at the Hillslope Scale in Drylands Using Structural Trait (De)composite. 

Eva Arnau-Rosalen, Emilio Rodriguez-Caballero, Angel Marques-Mateu, Matilde Balaguer-Puig, Jorge Lopez-Carratala, Adolfo Calvo-Cases, Roberto Lazaro-Suau, and Elias Symeonakis

Hydrological connectivity at the hillslope scale is a complex, spatially explicit phenomenon where surface and subsurface processes converge and interact, including infiltration, runoff, and lateral flow occurring during a singular rainfall event under specific antecedent soil moisture conditions.

In drylands, where Hortonian runoff generation prevails, such complexity has been conceptually simplified for operational purposes by using connectivity as a proxy for assessing ecosystem "health" or land degradation. Grounded in the current source-sink paradigm, a binary scheme of vegetation (pure sinks) and bare (pure sources) areas is used to distribute potential overland flow according to topography. The connectivity character is then distilled through the concept of Flow Length, with different metrics proposed under this rationale.

Despite this operational simplicity, the quantification of connectivity has yet to reach a standardized status, hindering intercomparison studies and the establishment of assessment baselines for land degradation.

Within the same framework umbrella, we recognize its shortcomings and propose decomposing the connectivity issue into three spatially explicit traits, each representing distinct structural features that emerge at the hillslope scale. This analytical approach aims to separately evaluate the contributions of vegetation patterns and flow routing, without the constraint of the hillslope shape. Facing the challenge of integrating these traits into a unified, synthetic metric for assessing runoff connectivity, we discuss several alternatives. The study is conducted at the experimental site in Benidorm (Alicante, Spain), using UAS-derived orthophotos and DEMs, where lateral variations within a small catchment serve to test the suitability of the proposal. This methodological proposal aims to advance the conceptual discussion toward developing a standardized approach for runoff connectivity evaluation and to inform land degradation assessments in drylands.

How to cite: Arnau-Rosalen, E., Rodriguez-Caballero, E., Marques-Mateu, A., Balaguer-Puig, M., Lopez-Carratala, J., Calvo-Cases, A., Lazaro-Suau, R., and Symeonakis, E.: Towards Standardising Runoff Connectivity Assessment at the Hillslope Scale in Drylands Using Structural Trait (De)composite., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19726, https://doi.org/10.5194/egusphere-egu25-19726, 2025.

EGU25-20458 | Orals | ITS4.20/NP0.4

 Vegetation pattern formation and community assembly under drying climate trends 

Induja Pavithran, Michel Ferre, Bidesh Bera, Hannes Uecker, and Ehud Meron

Drying trends driven by climate change and water stress pose significant threats to ecosystem functioning and the services they provide to humanity. To better understand ecosystem response to drying trends, we study a mathematical model of plant communities that compete for water and light. We focus on two major responses to water stress: shifts in community composition to stress-tolerant species and spatial self-organization in periodic vegetation patterns. We calculate community bifurcation diagrams of spatially uniform and spatially periodic communities. The bifurcation diagram reveals that as precipitation decreases, spatially uniform community shift from fast-growing to stress-tolerant species. However,  a reverse shift back to fast-growing species occurs when a Turing bifurcation is traversed and patterns form. We further find that the inherent spatial plasticity of vegetation patterns, in terms of patch thinning along any periodic solution branch and patch dilution in transitions to longer-wavelength patterns, buffers further changes in the community composition, despite the drying trend, and yet increases the resilience to droughts. Response trajectories superimposed on community Busse-balloons highlight the roles of the initial pattern wavelength and of the rate of the drying trend in shaping the buffering community dynamics. We discuss the implications of these results for dryland pastures and crop production.

How to cite: Pavithran, I., Ferre, M., Bera, B., Uecker, H., and Meron, E.:  Vegetation pattern formation and community assembly under drying climate trends, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20458, https://doi.org/10.5194/egusphere-egu25-20458, 2025.

NP1 – Mathematics of Planet Earth

EGU25-1302 | ECS | Orals | NP1.1

Uncertainty propagation on satellite data for synthetic indicators 

Jessie Levillain and Nicolas Gasnier

Combining satellite data from heterogeneous sources is often needed to produce synthetic indicators for natural resources and ecosystems. For instance, the temporal evolution of the water storage of a lake can be estimated by combining time series of satellite images (Sentinel-1, Sentinel-2) with measurements of the water surface elevation in 1D (nadir altimeters such as Sentinel-3 and 6) or 2D (swatch altimeter such as SWOT) and other available data.

These synthetic indicators are of great value for scientists, stakeholders, and policymakers, but quantifying their uncertainties bring new challenges. 

In the previous example, the estimation of the lake bathymetry is the most important stage as it determines the relationship between the observed water surface extent, the water surface elevation and the estimated relative water storage. 


We propose an optimal transport (OT)-based sensitivity analysis method to determine the probability distribution of the surface corresponding to the lake's observable bathymetry and the relative lake volume variations.
Taking two random variables X (known uncertainty input) and Y (unknown uncertainty output) on a measure probability space, along with their marginals ν and μ, we can define an OT-based global sensitivity measure between a sample Xa of X, and Y, based on the Wasserstein distance of order p between ν and μ.

Most sensitivity analysis methods only cater to the study of a univariate sensitivity measure, whereas using an OT-based sensitivity index allows the study of a multivariate response. Various metrics will be investigated in the presentation (Wasserstein-Bures metric, Wasserstein-Fréchet...) along with their advantages and drawbacks relatively to our multi-dimensional problem.

How to cite: Levillain, J. and Gasnier, N.: Uncertainty propagation on satellite data for synthetic indicators, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1302, https://doi.org/10.5194/egusphere-egu25-1302, 2025.

EGU25-2556 | ECS | Orals | NP1.1

Jacobi stability and aperiodicity of the Rikitake-Hide dynamo model based on KCC-theory 

Mitsuhiro Hirano, Hiroyuki Nagahama, and Takahiro Yajima

To understand the mechanisms underlying the magnetic fields of planets, including the Earth and the Sun, previous studies have proposed disk dynamo models as a suitable reduction of the mean-field dynamo equations. One of these is the Rikitake-Hide model, which combines the Rikitake model (a two-disk model for geomagnetic reversal) and the Hide model (a disk model with a motor and mechanical friction). This model reproduces nearly equal intervals of magnetic field reversals with modulated cycles, resembling the fluctuations of sunspots. In this presentation, we discuss the Jacobi stability and aperiodicity of the Rikitake-Hide model using geometrical invariants in the KCC (Kosambi–Cartan–Chern) theory. In the KCC theory, the second and third KCC invariants are related to the Jacobi stability and aperiodicity of trajectories in the system, expressed through variables (electrical currents and angular velocities) and parameters. By calculating the Jacobi stability of the Rikitake-Hide model using the second KCC invariant, we find that the model is Jacobi unstable when fluctuations in magnetic energy (square of the electric current) reach local minima. The instability at local minima manifests as branches in the trajectories of electric currents in the model. Based on the third KCC invariant for the trajectories of electric currents in the Rikitake-Hide model, the aperiodicity of the model may arise from individual electric currents. Although the model is always accompanied by aperiodicity, nearly equal intervals of magnetic field reversals are preserved through the cancellation of aperiodicity by symmetric cyclical fluctuations of electric currents. On the other hand, asymmetric electric currents originating from the motor and mechanical friction in the model alter the periods of magnetic field intervals. Finally, we consider the correspondence between the fluctuations of magnetic energy in the Rikitake-Hide model and sunspots on the Sun and discuss the implications for solar activity.

How to cite: Hirano, M., Nagahama, H., and Yajima, T.: Jacobi stability and aperiodicity of the Rikitake-Hide dynamo model based on KCC-theory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2556, https://doi.org/10.5194/egusphere-egu25-2556, 2025.

The Maximum Likelihood Ensemble Filter (MLEF) with State Space Localization (MLEF-SSL) was recently developed as a new ensemble data assimilation method that incorporates state space covariance localization in model space. The main motivation for developing this method was to enable global numerical optimization and assimilation of vertically integrated observations in an ensemble data assimilation system with covariance localization. MLEF-SSL uses random projection to compute the localized forecast error covariance and reduce the analysis dimensions to a manageable space. MLEF-SSL is being applied to a global NWP system named Nonhydrostatic Icosahedral Atmospheric Model (NICAM) with the assimilation of atmospheric observations, i.e., the NICAM-MLEF-SSL system, to explore its capability under a realistic high-dimensional dynamical application.

To apply MLEF-SSL in a high-dimensional system such as NICAM, a substantially large number of ensembles of the order of O(104) - O(105) is necessary to represent the localized forecast error covariance, thus, requiring special attention on the algorithmic development for the NICAM-MLEF-SSL system. This presentation will discuss the practical implementation of the NICAM-MLEF-SSL system on the RIKEN supercomputer Fugaku with an emphasis on the use of advanced math libraries for parallel computing.

In addition, the performance of NICAM-MLEF-SSL in assimilation of real atmospheric observations will be evaluated in detail and compared to that of NICAM-LETKF, which is the global data assimilation system that is currently used at RIKEN. 

Future plans related to the use of strong dynamical balance constraints and Artificial Intelligence (AI) techniques in NICAM-MLEF-SSL will also be discussed.

How to cite: Wu, T.-C., Zupanski, M., and Miyoshi, T.: Global Atmospheric Ensemble Data Assimilation using NICAM global icosahedral model and Maximum Likelihood Ensemble Filter with State Space Localization: Real Observation Experiment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2633, https://doi.org/10.5194/egusphere-egu25-2633, 2025.

EGU25-4017 | ECS | Posters on site | NP1.1

Finite-size local dimension as a tool for extracting geometrical properties of attractors of dynamical systems 

Martin Bonte and Stéphane Vannitsem

Local dimension computed using Extreme Value Theory (EVT) is usually used as a tool infer dynamical properties of a given state ζ of the chaotic attractor of the system. The dimension computed in this way is also known as the pointwise dimension in dynamical systems literature, and is defined using a limit for infinitely small neighborhood in the phase space around ζ. Since it is numerically impossible to achieve such limit, and because dynamical systems theory predicts that this local dimension is almost constant over the attractor, understanding the properties of this tool for a finite scale R is crucial. We show that the dimension can considerably depend on R, and this view differs from the usual one in geophysics literature, where it is often considered that there is one dimension for a given dynamical state or process. We also systematically assess the reliability of the computed dimension given the number of points to compute it.

This interpretation of the R-dependence of the local dimension is illustrated on the Lorenz 63 system for ρ = 28, but also in the intermittent case ρ = 166.5. The latter case shows how the dimension can be used to infer some geometrical properties of the attractor in phase space. The Lorenz 96 system with n = 50 dimensions is also used as a higher dimension example. A dataset of radar images of precipitation (the RADCLIM dataset) is finally considered, with the goal of relating the computed dimension to the (un)stability of a given rain field.

How to cite: Bonte, M. and Vannitsem, S.: Finite-size local dimension as a tool for extracting geometrical properties of attractors of dynamical systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4017, https://doi.org/10.5194/egusphere-egu25-4017, 2025.

Stochastic parameterisations are essential for representing the uncertainty introduced when numerical models neglect certain scales or components of the Earth system. Moreover, the specific structure of stochastic parameterisations is critical for representing this uncertainty accurately. A ubiquitous (though generally invalid) assumption is that of Markovianity. Computational constraints mean that Markovian parameterisations are much preferred in practice, but identifying optimal Markovian approximations is far from trivial. We propose an "online" data-driven approach to learning Markovian parameterisations, wherein the dynamics of the parameterised model feature explicitly in the loss function, which is based on a proper scoring rule. We apply the method to the problem of sub-grid closure of quasigeostrophic turbulence.

How to cite: Brolly, M. T.: Online learning of stochastic closures of quasigeostrophic turbulence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4165, https://doi.org/10.5194/egusphere-egu25-4165, 2025.

EGU25-4782 | ECS | Orals | NP1.1

Triggering inverse rotation in 1D model of blocky rock mass 

Maoqian Zhang, Arcady Dyskin, and Elena Pasternak

The weak connections between individual blocks in blocky rock mass lead to the possibility of block rotations. Rotation of non-spherical blocks pushes the adjacent blocks away; the phenomenon termed elbowing [1]. Furthermore, rotations in both directions create the lateral displacements in the same direction such that the behaviour becomes non-linear of absolute value type. In order to investigate the resulting pattern of elbowing blocks, we considered a simple one-dimensional structure (chain) of stiff square blocks holding together by springs. Only the end block (driving block) with a fixed centroid position is rotated, while each passive block has two degrees of freedom: translational and rotational. A one-dimensional physical model, analytical model, and numerical model (using the commercial discrete element software UDEC) are developed. It was observed that the passive blocks do not consistently rotate in the same direction as the driving block; instead, when the driving block reaches a certain critical angle, it triggers the change of the direction of rotation and the blocks start inverse rotation. We define the angle of the driving block, when the rotation of the passive blocks returns to zero, as the ‘angle of interior zero’. It was found that this angle is influenced by the magnitude of contact friction and the number of blocks. The result demonstrates the complexity of block motion pattern even in such a simple blocky system.

[1] Pasternak, E., Dyskin, A.V., Estrin, Y. (2006) Deformations in transform Faults with rotating crustal blocks. Pure Appl. Geophys. 163 2011-2030.

Acknowledgement: The authors are grateful to Dr I. Shufrin and the School of Engineering workshop for the help with designing and manufacturing of an initial version of the experimental device.

How to cite: Zhang, M., Dyskin, A., and Pasternak, E.: Triggering inverse rotation in 1D model of blocky rock mass, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4782, https://doi.org/10.5194/egusphere-egu25-4782, 2025.

EGU25-5113 | Orals | NP1.1

Laboratory study of hydraulic fracturing in heterogeneous materials 

Sergey Turuntaev, Evgeny Zenchenko, Tikhon Chumakov, and Petr Zenchenko

Real rocks are heterogeneous and contain cracks of various scales. The influence of these cracks on hydraulic fracturing was first studied in the 1980s, when experimental studies showed that the presence of natural fractures can affect the trajectory of the hydraulic fracture. Another type of inhomogeneous material is a homogeneous matrix with fragments of a different material with significantly different mechanical and filtration properties. By varying the composition and size of these fragments, it is possible to create samples with different characteristics. The interface between the matrix and the fragments acts as a weakened area, similar to cracks in a nonuniform fractured material.

Here we present the results of experiments conducted to study the propagation of hydraulic fracture in a heterogeneous material composed of a mixture of gypsum, cement, and fillers. Marbles chips and fine gravel were used as additives in the mixture. The porosity of the original samples without additives was 0.44 and the permeability was 4.15 mD. The porosity and permeability of samples with marble chips were 0.32 and 6.9 mD, respectively, while those with gravel were 0.30 and 2.74 mD. The height of the samples was 60 mm with an outer diameter of 104 mm. Brass inserts with an internal diameter of 10 mm and a length of 18 mm were placed in the center of both sides of each sample during manufacturing. The length of the uncased part of the well was approximately 24 mm.  The prepared sample was placed between two circular aluminum bases, with piezoelectric transducers mounted in the recessed working surfaces. Silicone liquid PMS-5, with a kinematic viscosity of 5 centistokes, was used to saturate the sample. During hydraulic fracturing, silicone liquid PMS-200, with a viscosity of 200 centistokes, was applied. The samples were subjected to radial stresses of 0.5 MPa, along the lateral surface, and axial stresses of 3 MPa were applied along the axis. The main focus of the experiments was on studying the acoustic emission accompanying the propagation of the hydraulic fracturing crack.

The experiments have shown that the presence of inclusions significantly affects the shape and development of hydraulic fractures: under conditions of radially symmetric lateral compression, fractures with three branches form in heterogeneous materials, while fractures with two wings form in homogenous samples. The fracturing pressure in samples with fillers is higher than in homogenous ones, and the highest fracturing pressure values are achieved when there is a more rigid and durable filler present. It has been established that acoustic emission pulses in an inhomogenous material have a wider frequency range than in a homogeneous one. In samples containing fillers, more acoustic emission pulses are recorded, especially when there are rigid fillers present. It is also worth noting that acoustic emission occurs earlier in experiments with homogenous samples relative to the time at which the maximum pressure is reached during hydraulic fracturing. The results of the acoustic emission source location are consistent with the observed patterns of cracks on the surface of the samples.

How to cite: Turuntaev, S., Zenchenko, E., Chumakov, T., and Zenchenko, P.: Laboratory study of hydraulic fracturing in heterogeneous materials, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5113, https://doi.org/10.5194/egusphere-egu25-5113, 2025.

EGU25-5131 | Posters on site | NP1.1

Defect-induced stress field triggering extensive tensile fracture growth in uniaxial compression 

Arcady Dyskin and Elena Pasternak

Mechanics of rock failure in uniaxial compression remains a challenge since the wing cracks produced by pre-existing defects/cracks in uniaxial compression are shown to wrap around the initial defect effectively arresting their further growth. As a result, they cannot grow to the extent sufficient for splitting rock samples. This presentation proposes another mechanism of rock failure based on extensive fracture growth caused by zones of tensile stresses formed as parts of self-equilibrating stress field induced by defects distributed in rock (both pre-existing and produced in the process of loading). The fracture driven by localised tensile stresses grows avoiding the zones of compressive stresses thus forming areas of interruption or overlapping. These areas work as distributed bridges constricting the fracture opening. Fractures with constricted opening have the stress intensity factors increasing with fracture growth making the fracture growth unstable and capable to break the rock.

Due to the necessity to avoid the compression zones the growing fracture will deviate form the straight path. If the sample size is not sufficiently large as compared to the size of the compression zones these deviations can be seen as inclined in one direction making the fracture oblique. This can be passed for the conventional shear fracture, which in fact cannot play a role in the process, as the shear fractures do not grow in their own plane forming wings instead. Therefore, the fractures observed in rocks failed in uniaxial compression, in both splitting and oblique failure types are tensile fractures with constricted opening formed and driven by the stress field induced by distributed defects. Whether the resulting failure is splitting or oblique (“shear” failure) depends upon the ratio of the sample size to the compression zones dimensions. We term this dependence “the scale effect in failure type”.

The proposed concept will form a basis for developing models of rock failure in compression necessary for analysing and predicting large scale failures in the rock mass, especially during mining operations.

How to cite: Dyskin, A. and Pasternak, E.: Defect-induced stress field triggering extensive tensile fracture growth in uniaxial compression, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5131, https://doi.org/10.5194/egusphere-egu25-5131, 2025.

EGU25-5137 | Posters on site | NP1.1

Rough fault with dilation. Triggering of full sliding 

Elena Pasternak and Arcady Dyskin

The presentation proposes a 2D model of sliding over a rough fault of finite length. Sliding over such a fault involves interaction between asperities of its opposite sides. The interaction proceeds in two stages. At Stage 1 (the initial stage) the interaction involves climbing asperities over the asperities on the opposite side of the fault, causing dilation. As a result, additional resistance to sliding is induced working as friction such that the friction angle becomes the sum of the material friction angle representing friction between the asperity contacts and the average angle of inclination of the tangential line of the asperity contacts. With the increase of shear stress above the critical value of the friction stress shear over the fault is initiated. This corresponds to the conventional interpretation of sliding over rough fault.

This conventional sliding however only proceeds until it reaches the half asperity length, that is when the corresponding local dilation (fault opening) reaches its maximum, which is the asperity height. Under uniform shear stress this is obviously reached at the fault centre. At this point Stage 2 commences. At Stage 2 the asperities which produced maximum dilation (the size of two asperity height) start reducing the dilation creating the effect of local negative friction since the pressure at this stage drives sliding. Subsequently, in the fault zone sliding in Stage 2 the average friction angle drops to that of the material friction angle. As a result, the central zone slides under reduced friction. It was found that there exists a critical magnitude of shear stress, which triggers self-sustained extension of the zone with reduced friction.

Sliding of this type involves creation of loci of negative friction, which can affect the microseismic signals. The presented model provides an additional mechanism of fault sliding and the associated induced seismicity.

How to cite: Pasternak, E. and Dyskin, A.: Rough fault with dilation. Triggering of full sliding, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5137, https://doi.org/10.5194/egusphere-egu25-5137, 2025.

EGU25-5286 | Orals | NP1.1

Multiscale PDE Models for Marginal Ice Zone Dynamics 

Kenneth Golden

Perhaps the most dynamic component of the Arctic sea ice cover is the marginal ice zone (MIZ), the transitional region between dense pack ice and open ocean. It widens severalfold and moves poleward in a dramatic annual cycle, impacting the climate system, ecological processes, and human accessibility to the Arctic. We’ll discuss multiscale partial differential equation models for MIZ dynamics and the sea ice concentration field. The MIZ is viewed as a liquid-solid phase transition region, or mushy layer, to obtain a model that captures the seasonal cycle. Parameters in the model depend on finer scale structure and are computed using rigorous homogenization methods. We also consider a related floe-scale model with advective forcing to study ice transport processes, jamming, and anomalous diffusion observed in ice floe GPS data.

How to cite: Golden, K.: Multiscale PDE Models for Marginal Ice Zone Dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5286, https://doi.org/10.5194/egusphere-egu25-5286, 2025.

Magnetotelluric (MT) sounding is a vital geophysical exploration method, renowned for its ability to investigate deep geological structures, detect low-resistivity anomalies, and support diverse applications. It is widely used in mineral and geothermal resource exploration, hydrogeological surveys, and deep structural studies, effectively delineating subsurface structures from hundreds of meters to hundreds of kilometers. However, MT inversion, essential for quantitatively analyzing subsurface electrical structures, faces challenges due to the inherent non-uniqueness of MT methods and noise in field data. Traditional deterministic inversion methods, which rely on gradient-based optimization, typically produce a single model or a set of models fitting the data but fail to quantify uncertainties, complicating interpretation and reducing reliability.

To address these challenges, this study adopts a Bayesian inference framework for MT inversion. Unlike deterministic methods, Bayesian inversion treats model parameters as random variables and iteratively updates their prior distributions using observational data, ultimately obtaining posterior probability distributions. This approach enables a quantitative assessment of inversion uncertainties. However, the computational demands of Bayesian inversion, particularly for 2D and 3D MT problems, pose significant challenges, with forward modeling efficiency being a critical bottleneck.

To overcome this, we propose an efficient MT forward modeling method based on the Extended Fourier Deep Operator Network (EFDO), a physics-informed neural operator network. EFDO leverages the principles of Fourier transforms and deep neural operator networks to learn the functional mapping between model conductivity inputs and MT forward responses. By embedding physical laws into the network, EFDO ensures accurate predictions while significantly improving computational efficiency. Once trained, EFDO predicts forward responses in milliseconds, achieving a speedup of 300 times compared to traditional Finite Volume Methods (FVM) while maintaining high accuracy. A multi-GPU distributed parallel training strategy further accelerates EFDO training, drastically reducing preparation time.

Additionally, we integrate Voronoi and Delaunay parameterization techniques with the reversible-jump Markov Chain Monte Carlo (rjMCMC) method to enhance model sampling efficiency. This establishes a robust 2D MT trans-dimensional Bayesian inversion framework. Numerical experiments and tests on the Coprod2 dataset demonstrate the method’s computational efficiency and reliability.

In summary, this study introduces a novel approach combining the physics-informed EFDO network and advanced parameterization techniques to improve efficiency and uncertainty quantification in MT Bayesian inversion, paving the way for rapid, high-dimensional geophysical exploration.

How to cite: Liao, W., Hu, X., and Peng, R.: Efficient 2D MT Forward Modeling and Trans-Dimensional Bayesian Inversion with Physics-Informed Neural Operator Networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7723, https://doi.org/10.5194/egusphere-egu25-7723, 2025.

EGU25-8234 | Posters on site | NP1.1

Local well-posedness of strong solution to a climate dynamic model with phase transformation of water vapor 

Jieqiong Ma, Ruxu Lian, and Qingcun Zeng

The primitive three-dimensional viscous equations for atmospheric dynamics with the phase transformation of water vapor are studied.
According to the actual physical process, we give the heating rate, mass of water, and precipitation rate, which are related to temperature and
pressure. In fact, in this system, the anelastic approximation is not used, and more complex boundary conditions and dissipation coefficients are given. Providing H2 initial data and boundary conditions with physical significance, we prove the local well-posedness of a unique strong solution to the moist atmospheric equations by the contractive mapping principle and the energy method in the H2 framework.

How to cite: Ma, J., Lian, R., and Zeng, Q.: Local well-posedness of strong solution to a climate dynamic model with phase transformation of water vapor, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8234, https://doi.org/10.5194/egusphere-egu25-8234, 2025.

EGU25-8388 | Orals | NP1.1

Advancing AI for Earth sciences with hybrid and causal models 

Gustau Camps-Valls

Understanding and predicting Earth system processes requires more than accurate forecasts—it demands uncovering the underlying relationships among variables and constructing models that are interpretable, physically consistent, and mathematically robust. While machine learning has demonstrated exceptional predictive capabilities, its models often neglect fundamental physical laws, raising concerns about reliability, interpretability, and trust. This work explores the integration of domain knowledge with machine learning through hybrid and causal modeling approaches, aiming to bridge data-driven insights with the principles of the physical sciences. By leveraging these methods, we can enhance our understanding of the data-generating processes and achieve results that are both consistent and explainable. I will present recent advances and strategies in this field, highlighting their potential to revolutionize Earth system research. This effort represents a step toward a long-term AI agenda for developing algorithms that drive knowledge discovery in Earth sciences.

 

https://arxiv.org/pdf/2010.09031.pdf

https://arxiv.org/abs/2104.05107.pdf

https://doi.org/10.1016/j.physrep.2023.10.005

How to cite: Camps-Valls, G.: Advancing AI for Earth sciences with hybrid and causal models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8388, https://doi.org/10.5194/egusphere-egu25-8388, 2025.

EGU25-8593 | Posters on site | NP1.1

Inverting Spanish NOx emissions using a neural network 

James Petticrew, Hervé Petetin, Isidre Mas Magre, Marc Guevara Vilardell, Oriol Jorba, and Carlos Pérez García-Pando

Air pollutant emissions represent key input information for modeling atmospheric chemical composition or evaluating air pollution control policies. Over the last decades, different approaches have been proposed for estimating emissions. These approaches include collecting activity data combined with emission factors to build bottom-up emission inventories, developing appropriate spatial and temporal disaggregation proxies applied to national or regional total estimates to construct top-down emission inventories, and creating complex data assimilation workflows around chemistry-transport models combined with observations to perform air pollution emission inverse modeling.

In the last decade, deep neural networks (DNNs) have demonstrated exceptional ability to model complex spatiotemporal data. Meanwhile, advances in Earth observation systems, such as the Tropospheric Monitoring Instrument (TROPOMI), have enabled the collection of high-resolution atmospheric composition data in near real-time. These developments open up opportunities to integrate the predictive power of DNNs with satellite observations to deliver rapid and accurate estimates of pollutant emissions in near real-time.

Deterministic CTMs offer insights into the forward relationship between emissions and atmospheric composition, and some studies are already suggesting that DNN might be able to estimate with reasonable predictive skills the chemical concentrations obtained from these physics-based models. While the forward mapping is well-defined, the inverse mapping—from atmospheric composition to emissions—is inherently ill-posed. Our objective is ultimately to exploit DNNs for doing air pollutant emission inverse modeling, without using the traditional data assimilation approach. This presents challenges, requiring the application of regularization techniques to address the ambiguity raised by this ill-posed problem.

Here, we will present the preliminary results of our study on training regularized DNNs for inverting the NOx emissions in Spain , utilizing training data derived from the MONARCH air quality model. We will take advantage of the flexibility offered by these models to create different training datasets and assess the performance of our models across different data scenarios.

 

How to cite: Petticrew, J., Petetin, H., Mas Magre, I., Guevara Vilardell, M., Jorba, O., and Pérez García-Pando, C.: Inverting Spanish NOx emissions using a neural network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8593, https://doi.org/10.5194/egusphere-egu25-8593, 2025.

EGU25-11928 | ECS | Orals | NP1.1

The Wind-Driven Double-Gyre Circulation: A topological characterization of attractors across regimes 

Nicolas Bodnariuk, Denisse Sciamarella, Sabrina Speich, Eric Simonnet, and Michael Ghil

We use a quasi-geostrophic model of the wind-driven double-gyre to explore qualitative changes in the system's behavior through a novel topological framework called Templex. This method characterizes and classifies the system's attractors in phase space across various regimes, from low-energy, temporally smooth dynamics to highly energetic and chaotic states. Our study focuses on stationary wind stress forcing to deepen the understanding of the underlying dynamics, starting from this simplified scenario to identify the physical processes involved, while the spatial resolution is gradually increased up to 5 km x 5 km.

The original system of partial differential equations describing the flow is converted into a set of ordinary differential equations using finite-difference methods. We take advantage of the Julia programming language to build the model, apply continuation methods, and perform stability analyses along the branches of a bifurcation tree, subject to pseudo-adiabatic variations in wind intensity. Our findings emphasize the effectiveness of topological methods in revealing the structural aspects of bifurcations, and in examining new pathways to study dynamical systems in geosciences. Moreover, we present novel insights on the existence of an attractor in the infinite-dimensional system, bridging the gap between topological results obtained numerically and the original mathematical model.

Through this presentation, we aim to foster discussion on the potential of topological approaches to advance the understanding of nonlinear systems in geophysical fluid dynamics.

How to cite: Bodnariuk, N., Sciamarella, D., Speich, S., Simonnet, E., and Ghil, M.: The Wind-Driven Double-Gyre Circulation: A topological characterization of attractors across regimes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11928, https://doi.org/10.5194/egusphere-egu25-11928, 2025.

EGU25-11939 | Posters on site | NP1.1

Estimation of Spatial-temporal Source Term of Chernobyl Wildfires using Deep Neural Network Prior 

Vaclav Smidl, Antonie Brozova, Ondrej Tichy, and Nikolaos Evangeliou

The source term of Chernobyl 2020 wildfires is a tensor consisting of five dimensions: spatial location described by longitude and latitude in a given area with potentially many sources, time profiles, height above ground level, and the size of particles carrying the material. Since the number of concentration measurements is limited, the estimation of this source term is an ill-posed problem. Prior information is thus essential to obtain a reproducible estimate. We show that deep image prior that utilizes the structure of a deep neural network to regularize the inversion is suitable for this problem. The deep network is initialized randomly without the need to train it on any dataset first. The networks is used to represent both the mean and variance of the posterior estimate. The resulting variational Bayes procedure thus introduces smoothness in the spatial estimate of the emissions and reduces the number of unknowns by enforcing a prior covariance structure in the source term. The estimate of the 137Cs emissions during the Chernobyl wildfires in 2020 is compared to the Tikhonov method. The spatial distribution of the proposed method is close to the distribution obtained from satellite observations. 

Acknowledgment: 
This research has been supported by the Czech Science Foundation (grant no. GA24-10400S). 

How to cite: Smidl, V., Brozova, A., Tichy, O., and Evangeliou, N.: Estimation of Spatial-temporal Source Term of Chernobyl Wildfires using Deep Neural Network Prior, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11939, https://doi.org/10.5194/egusphere-egu25-11939, 2025.

An important component of Earth's climate system is the land surface atmosphere interaction. For theoretical and empirical reasons, the strongest constraints to vegetation productivity, and thus drawdown of atmospheric CO2, as well as water use (evapotranspiration) are edaphic in nature. The appropriate treatment of the soil is related only to one of the topics listed in the call for abstract submissions, namely statistical mechanics. A new water balance treatment developed based on combining ecological optimality with distinct percolation scaling results for solute transport in directed as well as random networks as applied to root growth and soil formation delivers observed results for net primary productivity of vegetation, streamflow elasticity, evapotranspiration, plant species richness, and the scale dependence of the water cycle with a single parameter, which can be evaluated in a 2D or a 3D fractal model of plant roots. Most of the results summarized are generated from the 2D (thin soil) model, meaning that most of the above are consistent with predictions that use no adjustable or unknown parameters at all, merely their universal values from percolation theory.

How to cite: Hunt, A. G. and Ghanbarian, B.: With only stochastic and non-linear dynamics methods, the Earth surface component of climate cannot be modeled correctly, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12251, https://doi.org/10.5194/egusphere-egu25-12251, 2025.

EGU25-12270 | Orals | NP1.1

A topological perspective on the wind-driven ocean circulation 

Michael Ghil, Gisela Charó, Denisse Sciamarella, Juan Ruiz, and Stefano Pierini

We first present briefly recent insights on the effects of time-dependent forcing on systems with intrinsic variability, such as anthropogenic forcing on the climate system. These insights are applied next to the problem of periodic forcing of the wind-driven double-gyre problem. The topological perspective here is provided by applying recent advances in the algebraic topology of autonomously chaotic dynamic systems subject to time-dependent forcing. These advances are applied to the problem at hand.

The application starts by finding a topological representation of the underlying structure of the system’s flow in phase space by the construction of a cell complex that approximates its branched manifold and of a directed graph on this complex. The directed graph corresponds to the way that the flow in phase space moves from one cell of the complex to another.

Fundamental ingredients of the above representation, called generatexes and stripexes, delineate distinct ways of following the dynamical paths on the complex, namely the nonequivalent ways of travelling through the flow in phase space. These mathematically defined pathways will be shown to correspond to physical modes of variability.

How to cite: Ghil, M., Charó, G., Sciamarella, D., Ruiz, J., and Pierini, S.: A topological perspective on the wind-driven ocean circulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12270, https://doi.org/10.5194/egusphere-egu25-12270, 2025.

EGU25-13502 | Orals | NP1.1

A geometric interpretation of analysis 

Richard Ménard, Martin Deshaies-Jacques, and Annika Vogel

By its simplicity and intuitive appeal, the geometric interpretation of analysis provides a complementary understanding of minimum variance estimation.  The geometric interpretation is made possible by using a Hilbert space representation of random variables.  In this presentation we will argue how actually a geometric approach can help to explore/discover new relationships, in identifying assumptions, and provide an alternative pathway of understanding the concept of analysis and estimation of error covariances.  
For example, relationships between analysis increments in cross-validation could be easily derived.  An interpretation of sequential observation processing also follows a simple interpretation.  Important considerations in establishing relationships for an arbitrary number of collocated data sets could also be established.  Then we examine how we can relax the assumption of an optimal analysis.  This will guide us in deriving a new diagnostic of observation statistics with correlated errors.  

How to cite: Ménard, R., Deshaies-Jacques, M., and Vogel, A.: A geometric interpretation of analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13502, https://doi.org/10.5194/egusphere-egu25-13502, 2025.

EGU25-13518 | Orals | NP1.1 | Highlight

Natural variability-focused assessment of climate overshoot timing 

Josef Ludescher, Naiming Yuan, Hans Joachim Schellnhuber, and Armin Bunde

The Paris Agreement legally commits the international community to keep anthropogenic global warming well below 2.0°C, while major efforts shall be made to hold the 1.5°C-line. This is supported by ample scientific evidence indicating that climate change becomes difficult to manage beyond those lines due to highly nonlinear impacts (like tipping processes). The time range when the Paris guardrails will be transgressed under business as usual is highly relevant for precautionary adaptation measures and for justifying the rapid transformation towards a post-fossil economy. Fully-fledged Earth System Models (ESMs) are usually employed for the pertinent projections, yet they are not only computationally expensive but also lack explicit accounting for natural climate system variability. The latter may significantly distort (and invalidate) the ESM overshoot-timing projections. As an alternative, we present here a purely data-driven stochastic approach based on the persistence properties of the observed global temperatures. We are able to quantify, in a probabilistic way, the natural variability that must be superimposed on the anthropogenic trends in order to retrieve the observed warming behavior. When assuming that the anthropogenic warming continues at the current rate, we actually arrive at comparable overshoot timing estimates as the ESMs and provide an explanation for this finding.

How to cite: Ludescher, J., Yuan, N., Schellnhuber, H. J., and Bunde, A.: Natural variability-focused assessment of climate overshoot timing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13518, https://doi.org/10.5194/egusphere-egu25-13518, 2025.

EGU25-13544 | ECS | Orals | NP1.1

Hybrid data assimilation and machine learning algorithms for sparse observational data 

Sibo Cheng, Hongwei Fan, Yilin Zhuang, Tobias Sebastian Finn, Lya Lugon, Karine Sartelet, Karthik Duraisamy, Rossella Arcucci, and Marc Bocquet

Reconstructing spatiotemporal systems from sparse observations remains a long-standing challenge in several domains, including geoscience, air pollution and fluid dynamics. While various data assimilation (DA) and machine learning (ML) methods have shown potential, they still face significant challenges (see [1]): 

  • The computational burden of conventional DA algorithms (including error covariance specification), particularly for multivariate, high-dimensional systems.
  • Sparse and movable sensor placement, which makes conventional ML models (typically requiring fixed and regularly distributed input data) cumbersome.
  • The ill-defined nature of the sparse reconstruction problem, which poses significant risks of overfitting.

We will present our recent works aimed at addressing these challenges. More specifically, we developed latent DA algorithms [2] to reduce the computational burden of variational DA methods. These algorithms demonstrate great potential in efficiently assimilating sparse observations within a reduced-order latent space constructed by neural networks, thanks to the TorchDA library [3]. The latter enables GPU implementation of mainstream data assimilation methods and supports non-explicit state-observation transformation functions, provided they can be learned by a neural network.

We have also employed advanced deep learning techniques, including Voronoi-tessellation CNNs [4] and Vision Transformer-based autoencoders [5], to learn mappings from sparse observations to the complete physical space. These approaches effectively address challenges such as movable sensor placements and varying sensor numbers. Their integration with DA algorithms has also been evaluated.

Finally, our recent work explores [6] the utility of generative AI techniques, particularly denoising diffusion models, for field reconstruction from sparse observations. Generative AI methods offer two main advantages: first, they produce a sample from a probability distribution rather than predicting the mean as a fixed output, which can help mitigate overfitting caused by the illy-defined problem. Second, they inherently function as ensemble predictors by generating several samples, facilitating uncertainty quantification, which is essential in data assimilation. The numerical results tested on cases ranging from fluid dynamics benchmarks to semi-operational air pollution simulations will also be discussed.

[1] Cheng, S., Quilodrán-Casas, C., Ouala, S., Farchi, A., Liu, C., Tandeo, P., Fablet, R., Lucor, D., Iooss, B., Brajard, J., Xiao, D., Janjic, T., Ding, W., Guo, Y., Carrassi, A., Bocquet, M. and Arcucci, R, 2023. Machine learning with data assimilation and uncertainty quantification for dynamical systems: a review. IEEE/CAA Journal of Automatica Sinica

[2] Cheng, S., Chen, J., Anastasiou, C., Angeli, P., Matar, O.K., Guo, Y.K., Pain, C.C. and Arcucci, R., 2023. Generalised latent assimilation in heterogeneous reduced spaces with machine learning surrogate models. Journal of Scientific Computing

[3] Cheng, S., Min, J., Liu, C. and Arcucci, R., 2025. TorchDA: A Python package for performing data assimilation with deep learning forward and transformation functions. Computer Physics Communications

[4] Cheng, S., Liu, C., Guo, Y. and Arcucci, R., 2024. Efficient deep data assimilation with sparse observations and time-varying sensors. Journal of Computational Physics

[5] Fan, H., Cheng, S., de Nazelle, A.J. and Arcucci, R., 2024. ViTAE-SL: a vision transformer-based autoencoder and spatial interpolation learner for field reconstruction. Computer Physics Communications 

[6] Zhuang, Y., Cheng, S. and Duraisamy, K., 2025. Spatially-aware diffusion models with cross-attention for global field reconstruction with sparse observations. Computer Methods in Applied Mechanics and Engineering

How to cite: Cheng, S., Fan, H., Zhuang, Y., Finn, T. S., Lugon, L., Sartelet, K., Duraisamy, K., Arcucci, R., and Bocquet, M.: Hybrid data assimilation and machine learning algorithms for sparse observational data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13544, https://doi.org/10.5194/egusphere-egu25-13544, 2025.

EGU25-13641 | ECS | Posters on site | NP1.1

Scalable Approaches for Hierarchical Non-Gaussian Inverse Modelling for Emissions Estimation 

Stephen Pearson, Luke Western, Anita Ganesan, and Matt Rigby

Bayesian inverse modelling systems are a valuable tool for quantifying sources and sinks of greenhouse gases using atmospheric observations. They are increasingly used to verify national emission inventories submitted to the United Nations Framework Convention on Climate Change (UNFCCC). Recent studies have noted the value of hierarchical Bayesian inverse methods for improved uncertainty quantification in inverse modelling systems, and the importance of including physical constraints such as non-negativity in emissions. However, systems that exhibit these properties can suffer from severe computational bottlenecks, exacerbated by the growing volume of atmospheric observations and the demand for higher spatiotemporal resolution in emission estimates. As a result, spatial dimension reduction and spatiotemporal independence are often placed on emissions estimates, to make the algorithms computationally feasible. This research aims to explore these limits, before introducing novel approaches to address them.

We use a hierarchical Bayesian approach, using Markov chain Monte Carlo (MCMC) sampling, to explore the limits of the spatiotemporal resolution of flux estimates considering different multivariate Gaussian correlations. We demonstrate this by quantifying emissions of methane in the UK. In addition, we demonstrate the utility of a multivariate log-normal emissions distribution, simultaneously maintaining the non-negativity of emissions, as well as the explicit representation of emissions covariance. The results are compared with the emissions calculated using a spatially and temporally independent emissions prior, demonstrating the developments associated with a multivariate approach.

The computational costs associated with MCMC sampling means that the potential for extending the approach to large spatiotemporal parameter spaces is limited. Therefore, alternative inferential methods are explored, with a focus on sequential algorithms - such as Kalman filtering - that are augmented for non-Gaussian, hierarchal inference, in higher dimensional parameter spaces. This work provides the foundation for developing scalable non-Gaussian hierarchical frameworks that combine computational feasibility with improved emissions estimates.

How to cite: Pearson, S., Western, L., Ganesan, A., and Rigby, M.: Scalable Approaches for Hierarchical Non-Gaussian Inverse Modelling for Emissions Estimation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13641, https://doi.org/10.5194/egusphere-egu25-13641, 2025.

EGU25-13822 | Posters on site | NP1.1

Normal mode interactions in the Madden Julian Oscillation envelope 

Breno Raphaldini, Andre S. W. Teruya, Victor Mayta, Carlos F.M. Raupp, Pedro Dias, and Pedro Peixoto

The Madden Julian Oscillation (MJO) is the dominant element of the atmospheric variability  in the tropics on intraseasonal zonal timescales. The MJO manifests itself as a slowly eastward propagating envelope coupling large scale circulation and convection. Despite recent progress in the understanding of the MJO, a comprehensive theory of the MJO is still missing, partly due to its complexity associated with moist physics and nonlinearity.
Here, we use a normal mode decomposition of atmospheric reanalysis datasets to show that the MJO can be understood in terms of a superposition of interacting Rossby, Kelvin  and inertio-gravity modes. We discuss the nature of the interaction between these modes, which can be either linear, due to large-scale variations in the moisture, or simply due to the inherent nonlinearity of the equations of the atmosphere.  

How to cite: Raphaldini, B., S. W. Teruya, A., Mayta, V., F.M. Raupp, C., Dias, P., and Peixoto, P.: Normal mode interactions in the Madden Julian Oscillation envelope, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13822, https://doi.org/10.5194/egusphere-egu25-13822, 2025.

EGU25-14623 | ECS | Orals | NP1.1

Influence of loading control on tensile strength of rocks  

S v Dharani Raj, Thanh nhan Nguyen, Zili Huang, Giang d Nguyen, Murat Karakus, Ha h Bui, and Dat Phan

Snapback, a post-peak response often observed in brittle rocks, is crucial for accurately characterising fracture properties, particularly regarding size and strain rate effects. This study emphasises the application of the AUSBIT method, which utilises an indirect control approach, to maintain strain rate inside the fracture process zone (FPZ) within the quasi-static range. By selecting different specimen sizes, the AUSBIT technique effectively captures the snapback response while minimising dynamic effects.

The experimental results reveal significant variations in tensile strength measured using the AUSBIT method compared to traditional Brazilian Disc testing. This discrepancy highlights the effectiveness of AUSBIT in accurately reflecting the underlying fracture mechanisms through indirect strain-rate control. These findings offer important insights into rock fracture behaviours and support the potential of AUSBIT as a valuable tool for studying size and rate effects in brittle materials.

How to cite: Dharani Raj, S. V., Nguyen, T. N., Huang, Z., Nguyen, G. D., Karakus, M., Bui, H. H., and Phan, D.: Influence of loading control on tensile strength of rocks , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14623, https://doi.org/10.5194/egusphere-egu25-14623, 2025.

Sampling error is a fundamental limitation of assimilation schemes, such as the EnKF, that employ the sample covariance from an ensemble of forecasts.  Despite the fact that the EnKF is typically applied in situations where the ensemble size is small compared to the system dimension, most of what is known about the effect of sampling error comes from low-dimensional examples or asymptotic results valid when the ensemble size is large. For high-dimensional systems and small ensembles, progress can be made by leveraging (i) the diagonal form of the Kalman-filter update in the optimal coordinates of Snyder and Hakim (2022) and (ii) basic approximations from the theory of random matrices. These yield novel, explicit expressions for the EnKF gain, the (sample) mean and covariance of the EnKF posterior ensemble, and the error covariance of that posterior mean. The expressions show that a single EnKF update will remove almost all variance from the ensemble, unless the observations are very uninformative.  They also identify those directions in the state space for which the EnKF update is effective, improving the state estimate despite sampling errors, and those directions for which sampling errors in the EnKF overwhelm observational information and degrade the state estimate.

How to cite: Snyder, C.: Sampling error in the ensemble Kalman filter for small ensembles and high-dimensional states, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14641, https://doi.org/10.5194/egusphere-egu25-14641, 2025.

Abstract: With the continuous advancement of tunnel construction in cold regions, the shotcrete technique has been widely utilized in tunnel support, forming a concrete-rock composite structure. Influenced by the low-temperature climate in the cold region, the freezing of moisture around the tunnel will exert a significant frost heaving force on this structure, resulting in various degrees of freeze-thaw damage to the structure. Hence, investigating the damage characteristics of the rock-mass concrete material under freeze-thaw cycling conditions is of great significance for the protection of tunnel lining. In this study, an environmental scanning electron microscope (ESEM) test was conducted on the rock-concrete composites specimens, and the micro-damage deterioration mechanism and failure mode of the specimens subjected to uniaxial compression freeze-thaw cycling were analyzed from a microscopic perspective. The test results indicate that: (1) The freeze-thaw cycling causes irreversible damage to the interface area between the rock and concrete, with the number and length of micro-cracks continuously increasing, leading to the fracture and separation of some areas at the interface between the two. It directly affects the macroscopic mechanical performance of the specimens. (2) The freeze-thaw cycling weakens the cementation between particles. It can cause the structure between mineral particles to become loose, resulting in mineral shedding and fracture. Some fibrous minerals are damaged, and the size and quantity of pore structures continuously increase, while the integrity and bonding degree of minerals are damaged. (3) The composite specimens mainly experience splitting failure, sliding failure, and the combined mixed failure under uniaxial compression conditions. The splitting failure belongs to the tensile-shear failure dominated by tensile failure, and the sliding failure is a simple shear failure. Additionally, it is found that the interface failure mode of composite specimens (the inclination angle is 90°) is the tensile-shear failure dominated by tensile failure.

Key words: ESEM; freeze-thaw cycles; rock-concrete specimen; uniaxial compression

How to cite: Zhou, Z., Li, Y., Hu, Y., and Li, K.: Microscopic Deterioration Mechanism and Failure Mode of Rock-Concrete Composites Subjected to Uniaxial Compression and Freeze-Thaw Cycles using ESEM Technology , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15099, https://doi.org/10.5194/egusphere-egu25-15099, 2025.

EGU25-15195 | ECS | Orals | NP1.1

Teleconnection of Extreme Rainfall Events between the Yellow River Basin and Europe: A Complex Network Analysis 

Lin Cai, Naiming Yuan, Niklas Boers, and Jürgen Kurths

Extreme rainfall events (EREs) have recently been observed to exhibit teleconnection patterns across long spatial distances. Here we investigate the EREs over the Yellow River basin (YRB) using complex network-based event synchronization analysis. We found that EREs in the YRB are significantly synchronized with multiple regions worldwide, including both local regions and remote regions, and the spatial synchronization patterns exhibit time-scale dependence. Particularly, we found significant synchronization between the EREs in the YRB and those in Europe, with the YRB lags Eastern Europe by 3-5 days lag, while the YRB lags Western Europe by 5–7 days lag. Further analysis reveals that Rossby wave propagation plays a key role in the synchronization of EREs between Europe and the YRB. Wave trains originating in Europe propagate downstream of the Eurasian jet, inducing anomalous circulations over the YRB that enhance vertical upward motion and moisture transport, ultimately triggering EREs. Two distinct wave trains are observed across the Eurasian continent: one associated with Eastern Europe-YRB synchronization, occurring in the mid-latitude region and resembling Rossby wave patterns along the mid-latitude jet stream, with wave energy reaching the YRB after approximately 3 days; and another associated with Western Europe-YRB synchronization, positioned at higher latitudes and relates to Rossby waves along the polar front jet, with wave energy reaching the YRB in about 5 days. Our findings provide valuable insights into the predictability of EREs, offering critical guidance for improving forecasting and early warning capabilities for EREs in the YRB.

How to cite: Cai, L., Yuan, N., Boers, N., and Kurths, J.: Teleconnection of Extreme Rainfall Events between the Yellow River Basin and Europe: A Complex Network Analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15195, https://doi.org/10.5194/egusphere-egu25-15195, 2025.

EGU25-15845 | ECS | Orals | NP1.1

The DSI - a dynamic weather and climate index 

Annette Rudolph, Schielicke Lisa, Névir Peter, Trude Storelvmo, and Nikki Vercauteren

The Dynamic State Index (DSI) is a scalar diagnostic field that indicates deviations from a steady, adiabatic and inviscid atmospheric basic state. It is defined as Jacobian determinant of the potential voticity, the Bernoulli stream function and the potential temperature. Several works have been demonstrated that the DSI provides a suitable parameter to indicate diabatic processes across all scales. So far, DSI variants for different atmospheric models have been derived and applied to diagnose e.g. the onset and presence of precipitation or the organization of storms. In a novel approach DSI variants that identify specific polytropic states (isobaric, isochoric, isentropic, isothermal) of the atmosphere can be used for an analysis of cloud processes at different climate zones.

How to cite: Rudolph, A., Lisa, S., Peter, N., Storelvmo, T., and Vercauteren, N.: The DSI - a dynamic weather and climate index, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15845, https://doi.org/10.5194/egusphere-egu25-15845, 2025.

EGU25-16805 | ECS | Posters on site | NP1.1

Flow-dependent large-scale blending for limited-area ensemble assimilation 

Saori Nakashita and Takeshi Enomoto

Limited-area models (LAMs) often suffer from degradation in their representation of large-scale features compared to that of global models (GMs) due to the restricted domain size and limited observational coverage. To address this, we propose a novel flow-dependent large-scale blending (LSB) method for LAM data assimilation (DA). LSB methods incorporate large-scale information from a GM into the LAM DA system using scale-dependent weights. Our approach, termed as nested EnVar, extends the previously proposed static variational LSB method (nested 3DVar) to an ensemble-based framework. Unlike static LSB methods, nested EnVar simultaneously assimilates both observational and large-scale GM information into LAM forecasts with dynamically adjusting the weight given to GM information based on its estimated flow-dependent uncertainty. 

Through idealized assimilation experiments using a nested system of simplified chaotic models with a single spatial dimension, we demonstrate that nested EnVar effectively reduces large-scale errors in LAM DA as existing LSB methods, and offers better forecasts than GM downscaling. Compared to both traditional DA and other LSB methods, nested EnVar provides more accurate analyses and forecasts when dealing with dense and unevenly distributed observations. By dynamically accounting for GM uncertainty, nested EnVar improves the stability and accuracy of the analysis across scales. 

Our findings suggest that nested EnVar offers a promising alternative to traditional LSB methods for high-resolution simulations of complex, hierarchically structured phenomena. This novel approach has the potential to enhance the effectiveness of high-resolution LAM DA for spatially localized convective-scale observations.

How to cite: Nakashita, S. and Enomoto, T.: Flow-dependent large-scale blending for limited-area ensemble assimilation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16805, https://doi.org/10.5194/egusphere-egu25-16805, 2025.

EGU25-17167 | Orals | NP1.1

Transition process detection method of abrupt climate change 

Pengcheng Yan, Cailing Zhao, and Hong Li

Traditional abrupt climate change detection method often overlooks the process of the abrupt change. Considering the abrupt change process of climate change is conducive to further understanding the details of climate change. We propose the concept of the transition process of abrupt climate change and develop a climate transition process detection technology based on nonlinear models. Through dynamic segmented fitting, we identify the start time (state) and end time (state) of the abrupt change, as well as the stability parameters of the transition process, which are physical quantities that characterize the change process, and finely depict the characteristics of the transition process. Furthermore, based on the principle of critical slowing down, we derive generalized velocity and generalized force as early warning signals of abrupt climate change. During the change process, we also demonstrate the quantitative relationship between parameters during the system's change process, that is, the product of the degree of change stability and the square of the change amplitude is directly proportional to the change speed. This quantitative relationship has been confirmed in the observational data of global sea surface temperature. On this basis, prediction technology for climate turning points can be developed. This prediction technology has successfully predicted a transition process of the Pacific Decadal Oscillation.

How to cite: Yan, P., Zhao, C., and Li, H.: Transition process detection method of abrupt climate change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17167, https://doi.org/10.5194/egusphere-egu25-17167, 2025.

EGU25-18489 | ECS | Orals | NP1.1

The Dynamics of Jovian Polar Cyclones 

Laura Cope, Stephen Thomson, William Seviour, and Jemma Shipton

Polar vortices are observed in the atmospheres of most solar-system planets, arising as a single cyclone centred on or close to the pole. In contrast, Jupiter’s polar vortices have an unprecedented structure. As revealed by NASA’s Juno spacecraft, they consist of geometric patterns of cyclonic vortices surrounding a central cyclonic vortex at the pole. These crystalline structures were not predicted prior to being observed, and the mechanisms explaining their formation and evolution remain poorly understood. One possible mechanism is that moist convection produces small vortices in the polar regions, with the cyclones then migrating polewards via the ‘beta-drift’ mechanism and merging. Nevertheless, models including these processes do not spontaneously produce polygonal patterns like those on Jupiter. In contrast, this study investigates the stability of an initialized pattern of fully formed polar vortices subjected to these small-scale short-lived processes. This forced-dissipative system is modelled using the shallow-water equations describing a single layer of fluid on a polar gamma-plane. The initialized cyclones are subjected to a stochastic forcing with a short decorrelation time and the factors affecting their stability and time-evolution are studied. These include their degree of shielding (an anticyclonic ring around each cyclone), their depth and the properties of the forcing, in addition to the role of potential vorticity mixing.

How to cite: Cope, L., Thomson, S., Seviour, W., and Shipton, J.: The Dynamics of Jovian Polar Cyclones, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18489, https://doi.org/10.5194/egusphere-egu25-18489, 2025.

EGU25-18492 | ECS | Orals | NP1.1

Bridging the gap between Koopmanism and Response Theory: Using Natural Variability to predict Forced Response 

Niccolo' Zagli, John Moroney, Valerio Lucarini, Matthew Colbrook, and Igor Mezić

Complex chaotic systems exhibit nontrivial internal variability, with a power spectrum typically characterised by resonant broad peaks standing out on a continuous background of frequencies. These resonances correspond to nonlinear excitable modes of the system's evolution that can be generally attributed to long-lasting persistent events, weakly damped instabilities, or critical settings where the chaotic attractor is approaching a crisis [1].

In the context of the climate system, examples of such resonant behaviour are the El Niño Southern Oscillation, caused by a weakly damped instability of the atmosphere-ocean system [2], or the transition between the Warm and Snowball state of the Earth system due to a boundary crisis due to a change of the ice-albedo feedback [3].

On top of describing the relevant features of the internal variability of systems, such resonances also represent the fundamental modes shaping the resilience of the system to external perturbations. In particular, the linear response of the system to general forcing scenarios is solely determined by the Green’s function, for which a decomposition in terms of resonances can be obtained [4].

It is possible to establish a link between the system's nonlinear resonances and the spectral properties of the Koopman operator underlying the evolution in time of the system's observables.

Based on our work in [5], I will show that data-driven techniques developed to investigate the properties of the Koopman operator can be used to extract both resonances and dynamical modes from data. I will provide numerical evidence that the dynamical evolution of the statistical properties of the system can be interpreted as a superposition of such modes. In particular, by employing a projection of generic observables of the system onto the set of nonlinear modes, I will show that it is possible to reconstruct not only correlation functions but also the response of virtually any observable of interest.

Even though so far restricted to low dimensional systems, our results highlight the importance of such nonlinear modes in shaping the variability and response of chaotic systems and provide a way to (a) interpret the relevance of observables as a proxy to investigating dynamical properties of the system and (b) explain the difference between intrinsic variability of observables and their response to perturbations.

References

[1] Chekroun et al., Journal of Statistical Physics (2020) 179:1366–1402, https://doi.org/10.1007/s10955-020-02535-x

[2] Tantet et al., Journal of Statistical Physics (2020) 179:1449–1474, https://doi.org/10.1007/s10955-020-02526-y

[3] Tantet et al., 2018 Nonlinearity 31 2221, https://iopscience.iop.org/article/10.1088/1361-6544/aaaf42

[4] Manuel Santos Gutiérrez and Valerio Lucarini, 2022 J. Phys. A: Math. Theor. 55 425002, https://iopscience.iop.org/article/10.1088/1751-8121/ac90fd

[5] Zagli, Colbrook, Lucarini, Mezić, Moroney, “Bridging the gap between Koopmanism and Response Theory: Using Natural Variability to predict Forced Response”, https://doi.org/10.48550/arXiv.2410.01622

How to cite: Zagli, N., Moroney, J., Lucarini, V., Colbrook, M., and Mezić, I.: Bridging the gap between Koopmanism and Response Theory: Using Natural Variability to predict Forced Response, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18492, https://doi.org/10.5194/egusphere-egu25-18492, 2025.

EGU25-18862 | ECS | Orals | NP1.1

Characterization of dynamical properties and indicators of regime change in intermittent chaotic systems 

Alessandro Barone, Thomas Savary, Jonathan Demaeyer, Stéphane Vannitsem, and Alberto Carrassi

Intermittency has been initially linked to systems alternating regular and irregular states, while nowadays, it also encompasses systems that switch between two or more regimes. These include geophysical processes such as turbulence, convection, and precipitation patterns, not to mention applications in plasma physics, medicine, neuroscience, and economics. Traditionally, the study of intermittency has focused on global statistical indicators, such as the average frequency of regime changes under fixed conditions, or how these vary as a function of the system’s parameters or forcing, like in the case of climate change. However, these global indicators fail in capturing the local spatio-temporal nature of the regime transitions. 

In this work, we use  global and local perspectives to analyze intermittent systems and uncover reliable indicators of regimes’ changes. In particular, using tools such as the Lyapunov exponents and Covariant Lyapunov Vectors (CLVs), we have been able to characterize both global dynamics and local transitions in five different systems, of various complexities, and for three types of intermittency. We identified some key indicators and precursors of the regime transition that are common, despite the differences in the intermittency mechanism and in the dynamical model properties. At the same time, intermittency-type related mechanisms have been unveiled. For instance, we discover very peculiar behaviors in the Lorenz 96 (L96; Lorenz, 1996) and in the Kuramoto-Shivanshinki models (KS;  Kuramoto, Y. and Tsuzuki, T., 1976; G. Sivashinsky, 1977) that, despite their notoriety, have been so far unseen. In the L96 we identified crisis-induced intermittency with pseudo-periodic intermissions. In the KS equations we detected a spatially global intermittency which follows the scaling of type-I intermittency. 

In our local analysis, we uncover the relation between the CLVs mutual alignment and the regimes’ change, a connection that is present in all of the systems and for all types of intermittency considered. In the case of the on-off intermittency, the angle between CLVs is an effective precursor of the jump to the “on” regime. Furthermore, in all systems, the last CLV (the most stable), was found to carry important information about the dynamical features of the intermittency. In the case of type-I intermittency it allowed us to reconstruct the limit cycle around which the intermittency develops, in merging-crisis type of intermittency the last CLV successfully detected the pseudo-periodic intermissions, while in the case of on-off intermittency it allowed us to indicate the “off” state. 

The identification of these general and fundamental mechanisms driving intermittent behaviours, and in particular the detection of indicators spotting the regimes’ change, have the potential to be impactful in the study of turbulent geophysical fluids, rainfall patterns or atmospheric deep convection. In particular, they could be used to define a latent space of reduced dimension in which a neural network can be trained to automatically predict regime changes.

How to cite: Barone, A., Savary, T., Demaeyer, J., Vannitsem, S., and Carrassi, A.: Characterization of dynamical properties and indicators of regime change in intermittent chaotic systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18862, https://doi.org/10.5194/egusphere-egu25-18862, 2025.

EGU25-20158 | Posters on site | NP1.1

Flux Convergence and Divergence Linked to Asymmetric Transport by Large Turbulent Eddies  

Zhongming Gao, Lei Li, Heping Liu, and Bai Yang

It is well-established that large eddies significantly influence the turbulent transport of heat and scalars in the atmospheric surface layer. However, the mechanistic understanding of how large eddies originating from both the ground (updrafts) and aloft (downdrafts) regulate flux convergence (FC) and divergence (FD) remains relatively unexplored. Based on turbulence data measured at 12 levels, spanning from 1.2 m to 60.5 m above the ground, we observe a notable increase in the variability of sensible heat flux magnitudes with height. Our results show that FC and FD of sensible heat are primarily linked to variations in the respective transport efficiencies (RwT) at different heights. Using the cross-wavelet transform, we find that in FC cases, the regions with high wavelet coherence expand with height, resulting in higher RwT at higher levels compared to low ones. Conversely, in FD cases, the regions with high wavelet coherence decrease with height, leading to lower RwT at higher levels. Large eddies with length scales of approximately 120 to 500 m have a significant impact on amplifying or attenuating RwT at higher levels compared to lower levels. Using conditional sampling to extract the updrafts and downdrafts of large eddies, distinct patterns are observed in the characteristics of updrafts and downdrafts between FC and FD groups, especially in their flux contribution and transport efficiencies. This work emphasizes the significant contribution of asymmetric turbulent transport by updrafts and downdrafts to the discrepancy between the observed turbulent fluxes and those predicted by the Monin-Obukhov similarity theory.

How to cite: Gao, Z., Li, L., Liu, H., and Yang, B.: Flux Convergence and Divergence Linked to Asymmetric Transport by Large Turbulent Eddies , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20158, https://doi.org/10.5194/egusphere-egu25-20158, 2025.

EGU25-20233 | ECS | Orals | NP1.1

The chaotic tipping window and its dependence on relative timescales 

Raphael Roemer and Peter Ashwin

In the spirit of Hasselmann’s program, Climate Tipping Points are often studied in systems described by stochastic differential equations where a combination of noise and a parameter approaching or crossing a bifurcation threshold leads to tipping. However, in some cases, a multistable system forced by another potentially chaotic system is a more appropriate description and might give rise to unexpected effects.

We show how tipping in such chaotically forced systems is affected by varying the relative timescale between the chaotic forcing and the forced multistable system. Further, we explain how periodic orbits of the forcing system can help to understand this effect and how they can be used to characterise the chaotic tipping window.

How to cite: Roemer, R. and Ashwin, P.: The chaotic tipping window and its dependence on relative timescales, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20233, https://doi.org/10.5194/egusphere-egu25-20233, 2025.

Detecting subtle, spatially localized changes in climate datasets is essential for understanding evolving regional dynamics and extreme events—key topics in Earth and planetary sciences. We present EagleEye, a novel distribution-free approach for identifying local density anomalies between two multivariate datasets. By leveraging a nearest-neighbor strategy and a binomial-based test, EagleEye pinpoints regions of significant deviations without relying on complex model assumptions.

We illustrate its potential using temperature reanalysis products, where EagleEye reveals localized shifts in historical climate patterns—including notable positive anomalies around Greenland—that may indicate emerging changes in temperature fields. Owing to its scalability and interpretability, EagleEye can handle large, high-dimensional datasets and integrate multiple climatic variables within a single region. This framework offers an innovative avenue for probing evolving climate dynamics, highlighting areas undergoing rapid change, and supporting an enhanced understanding of climate variability—making it a valuable tool for geoscience applications and beyond.

How to cite: Springer, S.: EagleEye: Unsupervised Detection and Quantification of Local Density Anomalies in Climate Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21320, https://doi.org/10.5194/egusphere-egu25-21320, 2025.

EGU25-21616 | ECS | Posters on site | NP1.1

Typicality analysis for extreme climate events 

Vera Melinda Galfi

Recent studies found that the concept of typicality of extreme events is relevant in case of several weather and climate extremes related to atmospheric circulation anomalies, such as heatwaves or cold spells. This concept refers to the property of extreme events of being similar among each other while being at the same time anomalous with respect to usual weather conditions, referring to both spatial patterns and temporal evolutions. The aim of typicality analysis is to clarify whether this property applies to the extreme events of interest and to quantify the strength of typicality. In this presentation, I will discuss different types of typicality and give a practical guidance on how to perform a typicality analysis using climate datasets. I will present the most important steps of the analysis, discussing also several tools we can use to quantify typicality, such as standard statistical measures, Taylor diagrams, dynamical systems-based indicators.

How to cite: Galfi, V. M.: Typicality analysis for extreme climate events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21616, https://doi.org/10.5194/egusphere-egu25-21616, 2025.

EGU25-3877 | Orals | NP1.3

The Typicality of Regimes Associated with Northern Hemisphere Heatwaves 

Christopher Chapman, Didier Monselesan, James Risbey, Abdelwaheb Hannachi, Valerio Lucarini, and Richard Matear

We study the hemispheric to continental scale regimes that lead to summertime heatwaves in the Northern Hemisphere. By using a powerful data mining methodology -archetype analysis - we identify characteristic spatial patterns consisting of a blocking high pressure systems embedded within a meandering upper atmosphere circulation that is longitudinally modulated by coherent Rossby Wave Packets. Periods when these atmospheric regimes are strongly expressed correspond to large increases in the likelihood of extreme surface temperature. Most strikingly, these regimes are shown to be typical of surface extremes and frequently reoccur. Three well publicised heatwaves are studied in detail - the June-July 2003 western European heatwave, the August 2010 "Russian" heatwave, and the June 2021 "Heatdome" event across western North America. We discuss the implications of our work for long-range prediction or early warning, climate model assessment and post-event diagnosis.

How to cite: Chapman, C., Monselesan, D., Risbey, J., Hannachi, A., Lucarini, V., and Matear, R.: The Typicality of Regimes Associated with Northern Hemisphere Heatwaves, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3877, https://doi.org/10.5194/egusphere-egu25-3877, 2025.

EGU25-5631 | Orals | NP1.3

TurboMeter: attributing aviation turbulence events to climate change 

Tommaso Alberti, Lia Rapella, Erika Coppola, and Davide Faranda

Turbulence remains a pressing challenge for aviation safety and efficiency, as highlighted by recent incidents involving Singapore Airlines, Qatar Airways, and Scandinavian Airlines. Among the various types, Clear Air Turbulence (CAT) poses the greatest hazard due to its occurrence in clear skies, rendering it difficult to detect and predict. Furthermore, the unprecedented changes in Earth's climate are reshaping atmospheric dynamics on a global scale, with profound implications on aviation. As a companion of ClimaMeter, a platform designed to assess and contextualize extreme weather phenomena in relation to climate change, we introduce here TurboMeter. It is designed to use ERA5 reanalysis data to investigate the meteorological drivers of turbulence events by comparing them with historical analogues under similar atmospheric conditions. Turbulence diagnostics, including Ellrod’s indices, are used to evaluate the roles of jet streams, wind shear, and convective activity at typical cruising altitudes.

To illustrate TurboMeter, we present some recent aviation turbulence events occurred during 2024. Our findings reveal that they are closely linked to intensified jet streams and enhanced convective activity, influenced by the growing impacts of anthropogenic climate change. These results highlight a concerning trend: changing climatic patterns are altering the atmospheric drivers of turbulence, particularly CAT, with significant implications for flight safety and operational planning. Our study evidences the urgent need for improved weather forecasting and turbulence prediction models to mitigate aviation risks in a rapidly warming climate.

How to cite: Alberti, T., Rapella, L., Coppola, E., and Faranda, D.: TurboMeter: attributing aviation turbulence events to climate change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5631, https://doi.org/10.5194/egusphere-egu25-5631, 2025.

EGU25-5780 | Posters on site | NP1.3

ClimaMeter: a rapid attribution framework for weather extreme events 

Davide Faranda and the The ClimaMeter team
Climate change is a global challenge with manifold and widespread consequences, including the intensification and increased frequency of numerous extreme weather phenomena. In response to this pressing issue, we introduce ClimaMeter, a platform designed to assess and contextualize extreme weather phenomena in relation to climate change. The platform provides near-real-time information on the dynamics of extreme events, serving as a resource for researchers, policymakers, and acting as a scientific outreach tool for the general public. ClimaMeter currently analyzes heatwaves, cold spells, heavy precipitation, and windstorms.Our methodology is based on looking for weather conditions similar to those that caused the extreme event of interest with physics-informed machine-learning methodologies. We focus on the satellite era, namely the period since 1979, when widespread observations of climate variables from satellites have become available. The object studied (i.e. "the event") is asurface-pressure pattern over a certain region and averaged over a certain number of days, that has lead to a extreme weather conditions. We split the dataset 1979-Present in two parts of equal length and consider the first half of the satellite era  as "past" and the second part as "present" separately. We use data from MSWX. We then compare how the selected weather conditions have changed between the two periods, and whether such changes are likely due to natural climate variability or anthropogenic climate change.
This presentation sheds light on the methodology, data sources, and analytical techniques that ClimaMeter relies on, offering a comprehensive overview of its scientific foundations. To illustrate ClimaMeter, we present some examples of recent extreme weather events. Additionally, we highlight the role of ClimaMeter in promoting a profound understanding of the complex interactions between climate change and extreme weather phenomena, with the hope of ultimately contributing to informed decision-making and climate resilience. Follow us on the social-media @ClimaMeter and visit www.climameter.org.

How to cite: Faranda, D. and the The ClimaMeter team: ClimaMeter: a rapid attribution framework for weather extreme events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5780, https://doi.org/10.5194/egusphere-egu25-5780, 2025.

EGU25-7645 | ECS | Orals | NP1.3

Advancing the understanding of extreme events through the lens of dynamical system theory 

Chenyu Dong, Adriano Gualandi, Valerio Lucarini, and Gianmarco Mengaldo

Since Lorenz's pioneering work, dynamical systems theory has provided a powerful framework for studying complex systems. Among these, the study of their instantaneous properties is particularly significant for understanding short-lived yet impactful extreme events. Here, we propose an analogues-based index to measure the instantaneous predictability of dynamical systems over different forecasting horizons. We demonstrate its application in both classical dynamical systems and the Euro-Atlantic sector atmospheric circulation. Furthermore, recognizing that the onset of extreme events often involves processes operating across different scales, we introduce a novel framework that enables the exploration of scale-dependent dynamical properties. Given the flexible and generalizable nature of these methods, we believe they open new research avenues for studying extreme events from a dynamical systems perspective and will serve as valuable tools for deepening our understanding of extreme events.

How to cite: Dong, C., Gualandi, A., Lucarini, V., and Mengaldo, G.: Advancing the understanding of extreme events through the lens of dynamical system theory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7645, https://doi.org/10.5194/egusphere-egu25-7645, 2025.

EGU25-7685 | Orals | NP1.3

Progress and Challenges in the Study of Extreme Weather 

Gianmarco Mengaldo

Extreme weather events, including heatwaves, extreme precipitation, tropical cyclones, and other hazards, pose significant risks to society and ecosystems. Recent advancements in observational techniques, numerical modeling, theoretical frameworks, and AI methods have greatly improved our understanding and prediction of extreme weather events. However, despite significant progress, key challenges remain unresolved, particularly in achieving a thorough understanding of the physical drivers of extreme events, improving the transparency of AI-based prediction methods, and evaluating the vulnerability and resilience of cities to their impacts. To address these challenges, we present various approaches drawn from different fields, including dynamical systems theory, explainable AI, and NLP-based methods. Given the flexible and generalizable nature of these methods, we believe they may pave the way toward more robust solutions for addressing the challenges posed by extreme weather events.

How to cite: Mengaldo, G.: Progress and Challenges in the Study of Extreme Weather, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7685, https://doi.org/10.5194/egusphere-egu25-7685, 2025.

Compound climate and weather extremes have received significant attention in recent years due to the increased risks that they pose to the environment, human societies, and the economy. While prior studies have identified associations between various hazards in disaster databases, investigations focussing on droughts and floods remain rare. In this study, we analyze the impacts of concurrent or sequential drought-flood extremes from two widely used disaster databases: the Emergency Events Database (EM-DAT) and its geocoded version (GDIS), as well as the DesInventar database. The analysis focuses on the period from 1960 to 2018, aligning with GDIS temporal coverage. We define concurrent or sequential hazards as instances where a flood occurs during a drought period or within four months following a drought.  


Our findings for the global extratropics reveal that the economic losses and the number of affected people resulting from the identified drought-flood events are two to eight times higher than those ascribed to isolated droughts or floods, with a confidence interval ranging from two to twelve. Specifically, in DesInventar, the impact ratio (the mean impact of concurrent or sequential events divided by the mean impact of isolated events) for indirectly affected individuals and financial losses is approximately three. In EM-DAT, the impact ratio reaches three for economic damages and eight for affected individuals. Furthermore, the impact ratios are notably higher in the last 30 years of the study period compared to earlier decades, emphasizing the increasing severity of the drought-flood compound events.


These results highlight the amplified negative impacts when droughts and floods occur concomitantly or sequentially, highlighting the need for more robust policies to address their socio-economic risks, particularly under changing climatic conditions.

How to cite: Worou, K. and Messori, G.: Amplified Socio-Economic Impacts of Concurrent or Sequential Drought-Flood Events: Insights from Disaster Databases (1960–2018), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8719, https://doi.org/10.5194/egusphere-egu25-8719, 2025.

EGU25-10235 | ECS | Orals | NP1.3

Assessing the impact of climate change on wildfire development: insights from analogues and regional climate models 

Chen Lu, Rita Nogherotto, Tommaso Alberti, Gabriele Messori, Erika Coppola, and Davide Faranda

Climate change is an ongoing process that is modifying weather patterns and influencing weather phenomena and extreme events such as heatwaves, droughts, and floods. In this study, we investigate whether climate change can also play a role in enhancing wildfires by focusing on a set of three recent wildfires in Europe (i.e., events occurred in Central Sweden in July 2018, France in July 2022, and in Sicily and Greece in July 2023). We employ the concept of analogues to assess the influence of climate change on the atmospheric conditions underlying wildfire development monitored through the fire weather index, by comparing past and present atmospheric patterns similar to those that occurred during the wildfire. Our analysis focuses on both reanalysis data and high-resolution regional climate models to attribute the observed changes and provide future projections. Our findings show that climate change has altered critical factors supporting wildfire development, such as temperature, humidity, and wind patterns. The results from our sample of three events point out that climate change has increased wildfire hazards in Europe, which is projected to further increase for similar fire weather conditions in the future.

How to cite: Lu, C., Nogherotto, R., Alberti, T., Messori, G., Coppola, E., and Faranda, D.: Assessing the impact of climate change on wildfire development: insights from analogues and regional climate models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10235, https://doi.org/10.5194/egusphere-egu25-10235, 2025.

EGU25-10570 | Posters on site | NP1.3

VORTEX project: The role of the polar vortex on the predictabIlity of extreme events in the Northern Hemisphere 

Carmen Alvarez-Castro, Cristina Peña-Ortiz, David Gallego, and Davide Faranda

Extreme weather and climate events, marked by unexpected and severe conditions at the edges of historical distributions, significantly impact human health, society, and ecosystems. With global warming driving an increase in the frequency and intensity of these extremes, there is an urgent need to enhance weather prediction beyond the typical 7–10-day range. Among the atmospheric and oceanic components studied for improving predictability, the stratosphere stands out due to its slower and more predictable changes, which can have persistent impacts on surface weather patterns.

Research has highlighted the stratosphere's role in driving weather and climate extremes, particularly in the extratropical Northern Hemisphere. Events involving a weak or strong stratospheric polar vortex can precede the occurrence of surface extremes, making the polar vortex a key link between stratospheric variability and surface climate predictability. While various studies have previously identified this teleconnection, the processes connecting anomalous vortex states to extreme surface events are not yet fully understood.

In VORTEX project we employ a methodology based on advancements in dynamical systems theory to explore the relationship between anomalous polar vortex states and extreme precipitation and temperature events. This approach characterizes each vortex-extreme event's recurrence, persistence, and predictability, providing dynamic insights that traditional methods cannot. By identifying the intrinsic predictability of stratospheric patterns tied to extremes, this methodology offers a pathway to improve sub-seasonal to seasonal climate models, focusing future efforts on better representing critical patterns that influence extreme weather.

How to cite: Alvarez-Castro, C., Peña-Ortiz, C., Gallego, D., and Faranda, D.: VORTEX project: The role of the polar vortex on the predictabIlity of extreme events in the Northern Hemisphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10570, https://doi.org/10.5194/egusphere-egu25-10570, 2025.

EGU25-10822 | ECS | Orals | NP1.3

Exploring a new methodology to quantify natural variability in conditional extreme event attribution 

Clara Naldesi, Mathieu Vrac, Nathalie Bertrand, and Davide Faranda

Anthropogenic climate change (ACC) is one of the most demanding challenges facing our society. The intensification and increased frequency of many extreme events due to ACC are among its most impactful consequences, threatening human health, infrastructure, and ecosystems. In this context, raising the awareness of the general public of the relationship between ACC, extremes, and associated impacts becomes a crucial task.

This work is grounded in attribution science and focuses on quantifying and understanding the influence of internal climate variability on extreme events. Among the many tools available for attribution, we use ClimaMeter [Faranda et al. 2023], a rapid framework designed to provide context for extreme events in relation to ACC. ClimaMeter’s approach emphasizes the dynamics associated with extreme events and identifies weather conditions similar to those characterizing the event of interest, leveraging the analogues methodology for conditional attribution [Yiou, 2014]. The analysis provided by such a framework enables the evaluation of significant changes over time of the event’s dynamics and associated meteorological hazards and links them to ACC.

An essential part of ClimaMeter’s methodology is quantifying the influence of natural variability relative to ACC in explaining the changes associated with the event. Specifically, three modes of Sea Surface Temperature variability are taken into account: the El Niño-Southern Oscillation, the Atlantic Multidecadal Oscillation and the Pacific Decadal Oscillation. These three modes are considered with equal weight and changes not explained by them are assumed to be due to ACC [Faranda et al., 2023]. While the methodology is rapid and easy to communicate, it also has some limitations. In this work, we investigate the implications of this approach. First, we test it on a pre-industrial simulation of the IPSL climate model to evaluate its performance under stationary climate conditions. Additionally, we explore a generalization of the current methodology, aiming to refine the quantification of natural variability by weighing the three modes based on the event region and associated hazard. This generalized approach has the potential to expand ClimaMeter’s methodology and provide new insights into the complex mechanisms linking natural variability and extremes.

How to cite: Naldesi, C., Vrac, M., Bertrand, N., and Faranda, D.: Exploring a new methodology to quantify natural variability in conditional extreme event attribution, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10822, https://doi.org/10.5194/egusphere-egu25-10822, 2025.

EGU25-10966 | ECS | Posters on site | NP1.3

Winter cyclones drive stronger surface wind extremes in the North Atlantic than in the Southern Ocean 

Aleksa Stanković and Rodrigo Caballero

Hemispheric symmetries, including those in zonal-mean eddy kinetic energy and in hemispheric-mean planetary albedo, are a characteristic feature of Earth’s climate. Whether such a symmetry also holds for extreme surface windspeeds driven by midlatitude cyclones is currently unclear. We address this question by focusing on the regions with the peak of storm tracks over the North Atlantic, North Pacific and Southern Ocean. We analyse reanalysis and satellite datasets and employ objectively calculated storm tracks to associate cyclones with surface winds they produce. Additionally, we check for existence of trends in extreme windspeeds of each basin. Results show a statistically distinguishable hemispheric asymmetry in extreme surface windspeeds, with the North Hemisphere having stronger extremes, driven primarily by extreme windspeeds occurring during winter and in proximity to cyclones. This implies that cyclones in the North Hemisphere drive stronger surface windspeed extremes than in the South Hemisphere. The North Hemisphere also has higher extreme windspeeds above the boundary layer (700 hPa), pointing to the role of large-scale processes in driving these differences. Lastly, trends in the extreme surface windspeeds across all basins are positive in the reanalysis dataset, and statistically significant in the North Pacific and Southern Ocean.

How to cite: Stanković, A. and Caballero, R.: Winter cyclones drive stronger surface wind extremes in the North Atlantic than in the Southern Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10966, https://doi.org/10.5194/egusphere-egu25-10966, 2025.

EGU25-12284 | ECS | Orals | NP1.3

Comparative predictability of eastern and western north pacific blocking events 

Anupama K Xavier, Oisín Hamilton, Davide Faranda, and Stéphane Vannitsem

North Pacific blocking patterns, defined by persistent high-pressure systems that disrupt atmospheric circulation, are pivotal elements of mid-latitude weather dynamics. These blocking events play a significant role in shaping regional weather extremes, such as prolonged cold spells or heatwaves, and can redirect storm tracks across the Pacific. For instance, the 2021 Pacific Northwest heatwave demonstrated the profound impact of blocking on terrestrial temperatures, where an upstream cyclone acted as a diabatic source of wave activity, intensifying the blocking system. This led to heat-trapping stable stratification, which elevated surface temperatures to unprecedented levels (Neal et al., 2022). Similarly, marine heatwaves in the Northeast Pacific have been linked to high-latitude blocking events, which weaken westerly winds, suppress southward Ekman transport, and enhance ocean stratification, thereby increasing sea surface temperatures (Niu et al., 2023). The predictability of North Pacific blocking events is governed by the intricate interplay of large-scale atmospheric dynamics, ocean-atmosphere interactions, and internal variability (Smith et al., 2020).

This study investigates the differences in predictability between eastern and western North Pacific blocking events, using a modified version of the Davini et al. (2012) blocking index to distinguish their geographical locations. Identified blocking events were tracked using a block-tracking algorithm until they dissipated. Predictability was assessed by identifying an analogue pair for each blocking event. Specifically, after classifying blocks as eastern or western, geopotential height maps for each event were compared to all other days in the dataset. The analogue pair for an event was defined as the day with the smallest root mean square (RMS) distance. Predictability was then evaluated by averaging the error evolution of the tracks between events in each analogue pair.

Using CMIP6 model simulations and ERA5 reanalysis data, the study revealed that eastern blocks are significantly more persistent and stable than their western counterparts. Eastern blocks exhibited longer durations and greater resistance to atmospheric variability, resulting in improved forecast accuracy. In contrast, western blocks were found to be more transient and challenging to predict due to their susceptibility to dynamic instabilities.

References

Davini, P., Cagnazzo, C., Gualdi, S. and Navarra, A., 2012. Bidimensional diagnostics, variability, and trends of Northern Hemisphere blocking. Journal of Climate, 25(19), pp.6496-6509.

Neal, E., Huang, C.S. and Nakamura, N., 2022. The 2021 Pacific Northwest heat wave and associated blocking: Meteorology and the role of an upstream cyclone as a diabatic source of wave activity. Geophysical Research Letters, 49(8), p.e2021GL097699.

Niu, X., Chen, Y. and Le, C., 2023. Northeast Pacific marine heatwaves associated with high-latitude atmospheric blocking. Environmental Research Letters, 19(1), p.014025.

How to cite: K Xavier, A., Hamilton, O., Faranda, D., and Vannitsem, S.: Comparative predictability of eastern and western north pacific blocking events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12284, https://doi.org/10.5194/egusphere-egu25-12284, 2025.

EGU25-13213 | ECS | Orals | NP1.3

Sensitivity of Dynamical Coupling to Large-Scale Circulation in European Winter Extremes 

Ane Carina Reiter, Martin Drews, Gabriele Messori, Davide Faranda, and Morten Andreas Dahl Larsen

The physical mechanisms underlying climate-induced extreme events are inherently complex, arising from the compounding nature of multiple drivers and/or hazards. Leveraging the chaotic nature of the atmosphere, a novel approach, based on results from dynamical system theory, has recently been adopted to reveal the drivers of both individual and compound extremes. Central to this approach is the co-recurrence ratio, which quantifies the instantaneous dynamical coupling between multiple variables in terms of joint recurrences of atmospheric configurations to similar ones in the past.

While the co-recurrence ratio has demonstrated potential in revealing the atmospheric drivers of certain extremes, its performance may depend heavily on factors such as the choice of geographical domain(s), selection of variables, and the thresholds used to define extremes. These sensitivities remain underexplored, limiting the broader applicability of this approach.

In this study, we aim to address these gaps by assessing the sensitivity of the co-recurrence ratio in a European setting, focusing on daily winter extremes in temperature, wind, and precipitation. For this analysis, we adopt a bivariate focus, diagnosing the coupling between large-scale circulation patterns and single hazard variables.

By exploring these sensitivities, this work seeks to enhance the understanding of the robustness of the co-recurrence ratio and its effectiveness in diagnosing the atmospheric drivers of various types of extremes.

How to cite: Reiter, A. C., Drews, M., Messori, G., Faranda, D., and Dahl Larsen, M. A.: Sensitivity of Dynamical Coupling to Large-Scale Circulation in European Winter Extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13213, https://doi.org/10.5194/egusphere-egu25-13213, 2025.

EGU25-13374 | ECS | Posters on site | NP1.3

Causality and predictability of the Pan Atlantic compound extremes 

Meriem Krouma and Gabriele Messori

The co-occurrence of wintertime cold spells in North America and wet, windy extremes in Europe, known as the Pan-Atlantic compound extremes, is linked to distinct dynamical pathways. One of those dynamical pathways involves the presence of a persistent high-pressure system west of Greenland. This high-pressure anomaly tends to simultaneously induce a southward displacement of a trough over the eastern United States and sustain an upper-level trough over southwestern Europe, creating conditions that induce both cold spells in North America and extreme precipitation in Europe. The co-occurrence of the Pan-Atlantic compound extremes has been investigated in previous studies. However, the causal association between extremes on both sides of the Atlantic has yet to be verified. In this study, we aim to assess the relationship between these compound extremes and to uncover the causal mechanisms driving their co-occurrence. Preliminary findings indicate that high-pressure anomalies over Greenland are a main driver of both phenomena, providing a coherent dynamical link that bridges these geographically distinct extreme events. The study further seeks to clarify the underlying dynamics and improve predictability for such interconnected extreme weather events, which can help to better manage and mitigate their impacts.

How to cite: Krouma, M. and Messori, G.: Causality and predictability of the Pan Atlantic compound extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13374, https://doi.org/10.5194/egusphere-egu25-13374, 2025.

EGU25-13784 | ECS | Orals | NP1.3

RHITA: a framework for real-time detection and characterization of weather extremes 

Greta Cazzaniga, Adrien Burq, Mathieu Vrac, and Davide Faranda

Extreme weather events such as heatwaves, droughts, thunderstorms, and cyclones threaten human lives, ecosystems, and economic stability. Tracking and characterizing the spatiotemporal dynamics of such events is essential for understanding their cascading impacts on socioeconomic and environmental systems. When the detection and characterization of extremes are done in real-time, they can provide critical information that benefits many sectors, including agriculture, emergency management, and regulatory authorities.

To offer a tool for operational monitoring of weather-related hazards across Europe, we developed RHITA (Real-time Hazards Identification and Tracking Algorithm), an online framework designed for the rapid, automated, and objective spatiotemporal detection of hazards driven by extreme weather events. RHITA is intended for a wide range of users, including scientists, policymakers, authorities, and the general public. It leverages the ERA5 dataset for real-time detection, and the algorithm is calibrated using the EM-DAT dataset, which documents global disaster occurrences and impacts.

RHITA currently offers two main features: (1) real-time tracking and spatiotemporal characterization of extreme weather events such as heatwaves, droughts, cold spells, cyclones, and storms, focusing on associated hazards like extreme temperatures, water deficits, heavy precipitation, and strong winds; and (2) publicly available, up-to-date, transboundary historical spatiotemporal hazard catalogs for Europe.

How to cite: Cazzaniga, G., Burq, A., Vrac, M., and Faranda, D.: RHITA: a framework for real-time detection and characterization of weather extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13784, https://doi.org/10.5194/egusphere-egu25-13784, 2025.

EGU25-13891 | Posters on site | NP1.3

Ensemble Random Forest for Tropical Cyclone Tracking 

Pradeebane Vaittinada Ayar, Stella Bourdin, Davide Faranda, and Mathieu Vrac


Even though tropical cyclones (TCs) are well documented from the moment they reach a certain intensity to the moment they start to evanesce, many physical and statistical properties governing them are not well captured by gridded reanalysis or simulated by earth system models. Thus, the tracking of TCs remain a matter of interest for the investigation of observed and simulated tropical. Many cyclone tracking schemes are available. On the one hand, there are trackers that rely on physical and dynamical properties of the TCs and users prescribed thresholds, which make them rigid, and need numerous variables that are not always available in the models. On the other hand, there are trackers leaning on deep learning which, by nature, need large amounts of data and computing power. Besides, given the number of physical variables needed for the tracking, they can be prone to overfitting, which hinders their transferability to climate models. In this study, the ability of a Random Forest (RF) approach to track TCs with a limited number of aggregated variables is explored. Hence, it becomes a binary supervised classification problem of TC-free (zero) and TC (one) situations. Our analysis focuses on the Eastern North Pacific and North Atlantic basins, for which respectively 514 and 431 observed tropical cyclones tracks record are available from the IBTrACS database over the 1980-2021 period. For each 6-hourly time step, RF associates TC occurrence or absence (1 or 0) to atmospheric situations described by predictors extracted from the ERA5 reanalysis. Then situations with TC occurrences are joined for reconstructing TC trajectories. Results show good ability of the method for tracking of tropical cyclones over both basins and good ability for spatial and temporal generalization as well. It also shows similar TC detection rate as trackers based on TCs' properties and significantly lower false alarm rate. RF allows us to detect TC situations for a range of predictor combinations, which brings more flexibility than threshold based trackers. Last but not least, this study shed light on the most relevant variables allowing to detect tropical cyclone.

How to cite: Vaittinada Ayar, P., Bourdin, S., Faranda, D., and Vrac, M.: Ensemble Random Forest for Tropical Cyclone Tracking, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13891, https://doi.org/10.5194/egusphere-egu25-13891, 2025.

EGU25-14873 | ECS | Orals | NP1.3

Large-scale atmospheric circulation as a source of uncertainty in western European heat extreme projections  

Shutong Liu, Yinglin Tian, and Kai Kornhuber

Europe has been identified as a heatwave hotspot, where heatwave intensities have outpaced other mid-latitude regions in the Northern Hemisphere (Rousi et al. Nat. Comms. 2022). Accelerated European heatwave trends have been found to be associated with the increased persistence of Eurasian double jets, a specific set-up of the large-scale circulation in which the Northern hemisphere polar and subtropical jets occur as two clearly separated branches. However, if observed trends are projected to continue with anthropogenic warming and to what degree the present generation of climate models constitute useful tools to assess changes in the atmospheric circulation has not yet been ascertained.

In this study, we benchmark 11 CMIP6 climate models to evaluate their ability to reproduce the main characteristics of double jets and their relationship to heat extremes, aiming to identify the best-performing models for future projections. Our findings show that, on average, the models tend to underestimate the frequency of double jets by 80%. Moreover, half of the climate models underestimate the intensity of double-jet-associated heatwaves over Western Europe, with the remaining models even showing a negative anomaly in heatwave intensity during double jet events in the region. Furthermore, climate models fail to capture the growth rate of double jet persistence, with the model mean trend at -0.4 days per decade, while the observed rate is approximately 1.5 days per decade. The bias in the persistence trend of double jet in models is strongly correlated with the underestimation of the western European heat extreme trend, with an R2 value of 0.42.

Despite this, some models show reasonable agreement with the observations, and these models are further analyzed to project circulation-driven changes in extreme heat. Using EC-Earth3-Veg-LR, we observe an increase in double jet frequency from 2020 to 2060, at a rate of 0.2 days per decade. Our work highlights the need for better representation of double jet characteristics and their relationship with heat extremes in climate models to enhance preparedness for future heat risks.

How to cite: Liu, S., Tian, Y., and Kornhuber, K.: Large-scale atmospheric circulation as a source of uncertainty in western European heat extreme projections , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14873, https://doi.org/10.5194/egusphere-egu25-14873, 2025.

EGU25-15668 | ECS | Posters on site | NP1.3

High-risk atmospheric circulation patterns for Italian precipitation extremes 

Cristina Iacomino, Salvatore Pascale, Giuseppe Zappa, Marcello Iotti, Federico Grazzini, Alice Portal, and Paolo Ghinassi

Extreme precipitation events (EPEs) are meteorological phenomena that are likely to intensify as a result of climate change. They are a major concern for our society, especially in densely populated areas, as they can have significant economic and environmental impacts. Therefore, identifying large-scale atmospheric circulation that lead to EPEs is crucial for detecting geographical areas at risk and mitigating their adverse impacts.

To achieve this objective, we study the circulation patterns associated with EPEs in Italy. Initially, we focus on North-Central Italy and we identify the precipitation extremes in three datasets: ARCIS 3.0, MSWEP, and CERRA LAND. Circulation types associated with the EPEs are obtained by applying Self Organizing Maps (SOMs), an unsupervised artificial neural network widely used in synoptic climatology, to anomalies of geopotential height at 500 hPa and mean sea level pressure. Since ArCIS, the reference dataset, is limited to North-Central Italy, we extend the analysis to the whole of Italy using CERRA-Land. Such choice is based on the fact that it produced the most similar results to ArCIS in North-Central Italy compared to MSWEP.

We then generate composites of various variables (all retrieved from ERA5) for each SOM pattern to better understand the circulation patterns and characterize the atmospheric dynamics associated with extreme events. Additionally, we analyze the probability of exceeding the 99th percentile of wet-days to identify the areas impacted by each pattern. Composites for the different circulation types show variations in the synoptic pattern's position within the Mediterranean basin, as well as differences in the direction and intensity of moisture flux. These patterns influence distinct regions and display varying frequencies across seasons.

In future works the classification obtained by this study will be applied to climate model simulations, aiming to investigate the role of anthropogenic climate change in the dynamics leading to EPEs in Italy. 

How to cite: Iacomino, C., Pascale, S., Zappa, G., Iotti, M., Grazzini, F., Portal, A., and Ghinassi, P.: High-risk atmospheric circulation patterns for Italian precipitation extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15668, https://doi.org/10.5194/egusphere-egu25-15668, 2025.

EGU25-17645 | Orals | NP1.3

Graph neural networks based climate emulator for kilometer scale hourly precipitation : a novel hybrid imperfect approach 

Erika Coppola, Valentina Blasone, Serafina Di Gioia, Guido Sanguinetti, Viplove Arora, and Luca Bortolussi

Regional climate emulators provide computationally efficient tools for generating high-resolution climate projections, bridging the gap between coarse-scale models and the detailed resolution required for local-scale hazard assessments. Climate hazards from extreme precipitation events are projected to increase in frequency and intensity under global warming, emphasizing the need for accurate modeling of convective processes. However, traditional numerical methods are constrained by low resolution or the high computational costs of kilometer-scale simulations.

To overcome these limitations, we introduce GNN4CD, a novel deep learning emulator that estimates kilometer-scale (3 km) hourly precipitation from coarse atmospheric data (~25 km). The model leverages graph neural networks and a hybrid imperfect approach (HIA) for downscaling, initially trained on ERA5 reanalysis and observational data, and applied using regional climate model (RegCM) data for present-day and future projections.

GNN4CD demonstrates exceptional performance in reproducing precipitation distributions, seasonal diurnal cycles, and extreme percentiles across Italy, even when trained on northern Italy alone. The model captures shifts in precipitation distributions, particularly for extremes, across historical, mid-century, and end-of-century scenarios. Additionally, evaluations using an ensemble of convection-permitting regional models confirm GNN4CD's ability to replicate ensemble spreads for both present-day and future projections essential for estimating the uncertainty in the future climate change signal..

How to cite: Coppola, E., Blasone, V., Di Gioia, S., Sanguinetti, G., Arora, V., and Bortolussi, L.: Graph neural networks based climate emulator for kilometer scale hourly precipitation : a novel hybrid imperfect approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17645, https://doi.org/10.5194/egusphere-egu25-17645, 2025.

EGU25-17852 | ECS | Posters on site | NP1.3

The impact of the upward trend in the NAO index on precipitation dynamics in the Mediterranean region 

Emma Schultz, Barend Spanjers, and Dim Coumou

The North Atlantic Oscillation (NAO) is the dominant pattern of atmospheric variability over the North Atlantic region, having its greatest influence on Europe during the winter months. In winter, positive NAO index values are linked to warmer temperatures and increased precipitation in western and northern Europe, whereas southern Europe tends to experience colder and drier conditions. These drier conditions can pose significant challenges for agriculture and livelihoods. An overall positive trend in the NAO index has been observed in winter in recent decades. However, how precipitation dynamics in the Mediterranean region respond to the shift towards a higher NAO index are largely unknown, partly due to the poor capture of NAO’s upward shift in climate models. 

Here we examine the impact of the shift towards a higher NAO index on precipitation dynamics in the Mediterranean region in winter. We employ a novel statistical model to analyse next-day precipitation conditional on past observations. The analysis focuses on conditioning drought persistence on different NAO states to assess their influence on the distributional characteristics of drought durations across the Mediterranean region. We present preliminary analyses that contribute to the growing body of evidence that long-term positive trends in the NAO index have an impact on rainfall patterns and drought occurrence in Europe. Understanding the role of teleconnections in regional climate variability and long-term trends is essential for robust regional climate projections for improved risk assessment and policy planning.

How to cite: Schultz, E., Spanjers, B., and Coumou, D.: The impact of the upward trend in the NAO index on precipitation dynamics in the Mediterranean region, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17852, https://doi.org/10.5194/egusphere-egu25-17852, 2025.

EGU25-17937 | ECS | Orals | NP1.3

Impact Attribution for Climate Law: The Case of Storm Irene 

Mireia Ginesta, Shirin Ermis, Rupert Stuart-Smith, and Benjamin Franta

People are increasingly turning to courts to combat climate crisis. In the early 2000s, fewer than 10 climate change litigation cases had been filed globally. By 2024, this number has grown to over 2,500, with more than half originating in the United States. Some of these cases rely on extreme weather attribution science to link damages to anthropogenic climate change. Developing rigorous, legally useful assessments of damage attributable to climate change is an increasingly pressing need.

We present a framework for forecast-based impact attribution which can link physically consistent hazards to impacts, providing evidence for legal cases and climate cost recovery laws. As a case study, we analyze the severe impacts of Storm Irene in August 2011 when it was undergoing extratropical transition in the north-eastern USA. In the state of Vermont, Irene caused rainfall of up to 180 mm within a few hours, leading to fluvial and pluvial flooding with catastrophic consequences that caused $850 million in economic damages. By integrating an operational weather forecast model (ECMWF’s IFS) and hydrological models with economic impact assessments, we assess the extent to which these damages can be attributed to anthropogenic climate change.

This research underscores the potential of interdisciplinary attribution methodologies to enhance the scientific basis for judicial adjudication on climate change and climate law-making.

How to cite: Ginesta, M., Ermis, S., Stuart-Smith, R., and Franta, B.: Impact Attribution for Climate Law: The Case of Storm Irene, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17937, https://doi.org/10.5194/egusphere-egu25-17937, 2025.

EGU25-17947 | Orals | NP1.3

Towards an impact-based approach to the detection of analogues: the case study of Emilia-Romagna floods in May 2023 

Valerio Lembo, Mireia Ginesta, Tommaso Alberti, Roberta D'Agostino, and Davide Faranda

The framework of weather analogues is a powerful methodology for the detection of the climate change fingerprint on weather extremes, that has been widely used in several contexts. The procedure has several advantages compared to standard model-based attribution exercises, being fast and not computationally expensive. Here we address whether the detection of analogs based on impacts (e.g., environmental, socio-economic) of a severe weather event can provide added value on the attribution of the event intensity or likelihood to climate change.

As a case study, we analyse the twin Emilia-Romagna flood event of May 2023. It caused a sizable amount of casualties, widespread destruction and substantial economic damage. We detect analogues of the river runoff as an impact-based observable of interest, addressing it in an univariate context, but also jointly with other observables (i.e., in a multivariate framework), such as mean sea-level pressure, total precipitation, and 850 hPa vorticity. We therefore detect the optimal set of variables for performing multivariate analysis and the appropriate analysis domain. We suggest that by combining river runoff with other observables by carefully selecting the spatial domain, we obtain a clearer view of the role played by anthropogenic climate change for this event, also including the additional vulnerability linked to the environmental impact of human activities, such as land-use change and freshwater diversion.

How to cite: Lembo, V., Ginesta, M., Alberti, T., D'Agostino, R., and Faranda, D.: Towards an impact-based approach to the detection of analogues: the case study of Emilia-Romagna floods in May 2023, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17947, https://doi.org/10.5194/egusphere-egu25-17947, 2025.

EGU25-18710 | Orals | NP1.3

The predictable chaos of rare events in geophysical and complex systems 

Tommaso Alberti, Davide Faranda, and Valerio Lucarini

Many natural systems show emergent phenomena at different scales, leading to scaling regimes with signatures of chaos at large scales and an apparently random behavior at small scales. These features are usually investigated quantitatively by studying the properties of the underlying attractor. This multi-scale nature of natural systems makes it practically impossible to get a clear picture of the attracting set as it spans over a wide range of spatial scales and may even change in time due to non-stationary forcing.

Here we present a review of some recent advancements in characterizing the number of degrees of freedom and the predictability horizon of geophysical and complex systems showing non-hyperbolic chaos, randomness, state-dependent persistence and predictability. We compare classical approaches, based on Lyapunov exponents and correlation dimension, with novel approaches based on combining adaptive decomposition methods with concepts from extreme value theory. We demonstrate that the properties of the invariant set depend on the scale we are focusing on and that the proposed formalism can be generally helpful to investigate the role of multi-scale fluctuations within complex systems, allowing us to deal with the problem of characterizing the role of stochastic fluctuations across a wide range of physical systems as well as the role of different dynamical components in determining the predictability of rare events in complex systems.

How to cite: Alberti, T., Faranda, D., and Lucarini, V.: The predictable chaos of rare events in geophysical and complex systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18710, https://doi.org/10.5194/egusphere-egu25-18710, 2025.

EGU25-18740 | ECS | Orals | NP1.3

Analyzing the Historical and Projected Evolution of the Global Diurnal Temperature Range (DTR) 

Muskula Sai Bargav Reddy, Vinnarasi Rajendran, and Mukul Tewari

The Diurnal Temperature Range (DTR) serves as a crucial meteorological indicator, reflecting the difference between daily maximum and minimum temperatures and the magnitude of diurnal extremes. The anomalous values of DTR are often linked to the occurrence of various climatic extremes such as droughts, heatwaves, and wet spells, which make it necessary to understand the evolution of DTR both historically and for the future. This study focuses on analyzing the evolution of DTR globally by employing the non-stationary Multidimensional Ensemble Empirical Mode Decomposition (MEEMD) method. To accomplish this, historical temperature data spanning 69 years (1951-2019) and CMIP6 Bias corrected data covering 150 years (1951-2100) were utilized. The non-linear trend characteristics in temperature are computed using CRU 0.50 x 0.50 gridded temperature data for historical trends and five different bias-corrected climate projection datasets of NASA Earth Exchange Global Daily Downscaled Projections (NEX-GDDP-CMIP6) for the assessment of trends in future DTR by considering two SSP scenarios, i.e., SSP 245 and SSP 585, each corresponding to intermediate and high emissions scenarios. The CMIP6 models that are considered are CanESM5, GFDL CM4, MIROC6, NorESM2-MM, and MPI-ESM1-2-HR. The results from the analysis reveal the decrease in global DTR, with a faster rate of increase in minimum temperature than in maximum temperature. However, the southern regions of Australia and Africa showed an increase in DTR. The CMIP6 simulations showed that CanESM5 and MPI-ESM1-2-HR showed a decreasing trend in global DTR for both scenarios of ssp, with an increase in DTR for South America and the southern part of Africa for CanESM5, while GFDL CM4, MIROC6, and NorESM2-MM showed a decrease in global DTR. The findings underscore the importance of understanding regional climatic variations when assessing global temperature trends. The observed contrasting regional patterns in DTR highlight the influence of localized hydroclimatic factors, including land-use changes, aerosols, and atmospheric feedback mechanisms. These insights are crucial for refining climate models and improving future climate projections under different emission pathways. Overall, the study emphasizes the necessity of incorporating non-linear approaches like MEEMD to capture complex climatic trends and underscores the role of DTR as a key indicator of climate change and its impacts at both global and regional scales.

How to cite: Reddy, M. S. B., Rajendran, V., and Tewari, M.: Analyzing the Historical and Projected Evolution of the Global Diurnal Temperature Range (DTR), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18740, https://doi.org/10.5194/egusphere-egu25-18740, 2025.

EGU25-19577 * | Orals | NP1.3 | Highlight

Unraveling the Rising Threat of Atmospheric and Marine Heatwaves in the Mediterranean Region 

Samira Khodayar Pardo, Paco Pastor, and Laura Paredes-Fortuny

Heatwaves (HWs) are extreme climate events increasingly magnified under climate change, posing significant risks to both human and environmental systems. The Mediterranean region, recognized as a climate change hotspot, is experiencing a worrying amplification of both atmospheric and marine heatwaves. In this presentation we will discuss the evolution and interplay of these phenomena emphasizing their compounding effects when occurring simultaneously.

Our findings reveal a clear increase in HW frequency, intensity, and duration, with the concurrence of atmospheric and marine heatwaves resulting in a significant local amplification of marine heatwave intensity. While atmospheric heatwaves remain largely unaffected by this interaction. This interaction has become more prominent in recent years, highlighting the increasing complexity of extreme climate phenomena in this region.

The results underscore the urgent need for regionally tailored strategies to mitigate the cascading impacts of compounding heatwaves, as their intensification under climate change exacerbates threats to Mediterranean ecosystems and communities.

 

How to cite: Khodayar Pardo, S., Pastor, P., and Paredes-Fortuny, L.: Unraveling the Rising Threat of Atmospheric and Marine Heatwaves in the Mediterranean Region, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19577, https://doi.org/10.5194/egusphere-egu25-19577, 2025.

EGU25-19698 | Orals | NP1.3

 January 2025 Wildfires in Southern California are attributable to Anthropogenic Global Warming 

Rita Nogherotto, Chen Lu, Greta Cazzaniga, Coppola Erika, and Davide Faranda

Starting January 7, 2025, devastating wildfires have swept through the Los Angeles metropolitan area and nearby regions. By January 10, the fires had caused ten deaths, destroyed thousands of structures, displaced nearly 180,000 residents, and scorched approximately 30,000 acres. This study employs the extended ClimaMeter (climameter.org <http://climameter.org/>) protocol to explore the potential role of climate change in exacerbating the severity of this event. Specifically, we examine whether climate change has modified the atmospheric conditions, represented by the mean sea level pressure, that contribute to wildfire occurrence, represented by the fire weather index, by analyzing historical and current weather patterns similar to those observed during the fires. Our methodology integrates both reanalysis datasets and high-resolution regional climate models to assess observed changes and project future fire risk scenarios. The results indicate a significant increase in the fire weather index across much of California and surrounding regions, which suggests that this event can be ascribed to human-driven climate change. The models show a similar signal in the present climate and project increases in fire weather hazard in the future.

How to cite: Nogherotto, R., Lu, C., Cazzaniga, G., Erika, C., and Faranda, D.:  January 2025 Wildfires in Southern California are attributable to Anthropogenic Global Warming, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19698, https://doi.org/10.5194/egusphere-egu25-19698, 2025.

EGU25-20545 | ECS | Orals | NP1.3

Characterizing ENSO Through Topological Analysis of Jin-Timmermann Model's Chaotic Regimes 

Maria Sanchez Muniz, Margaret Brown, and Pushpi Paranamana

The El Niño-Southern Oscillation (ENSO) represents one of the most significant drivers of global climate variability. This study investigates the chaotic parameter regimes of the Jin-Timmermann model, particularly focusing on the dynamics identified by Guckenheimer et al. where chaotic attractors emerge. We analyze the reduced three-dimensional system with specific attention to the critical parameters δ = 0.225423, ρ = 0.3224, which govern the time-scale interactions between oceanic and atmospheric processes. Using topological data analysis (TDA), we characterize the structural transitions between periodic and chaotic behaviors in the model's parameter space. Our methodology combines persistent homology with dynamical systems theory to identify distinct topological signatures associated with strong El Niño events. We validate these theoretical findings against observational data from the ERA5 reanalysis and NOAA/ERSSTv5 Niño 3.4 index, focusing particularly on the relationship between topological features and prolonged dry conditions in Southeast Asia. This approach provides new insights into the non-systematic relationship between strong El Niño events and regional climate impacts, while establishing a novel framework for comparing theoretical models with observational data. Our results demonstrate the utility of topological methods in understanding complex climate phenomena and suggest new possibilities for improving ENSO prediction capabilities.

How to cite: Sanchez Muniz, M., Brown, M., and Paranamana, P.: Characterizing ENSO Through Topological Analysis of Jin-Timmermann Model's Chaotic Regimes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20545, https://doi.org/10.5194/egusphere-egu25-20545, 2025.

Extreme rainfall events during the Indian monsoon season pose significant challenges due to their socioeconomic and environmental impacts. Understanding the spatial and temporal dynamics of these events requires robust analytical and statistical methods capable of capturing complex relationships within rainfall generating systems. Complex network approaches have emerged as powerful tools for analyzing spatiotemporal patterns in climate data, offering new insights into extreme weather phenomena.

This study compares two methodologies for constructing and analyzing climate networks to study the spatiotemporal structure and dynamics of heavy precipitation events in India during the monsoon season across multiple time scales. Specifically, we introduce a novel combination of Discrete Wavelet Decomposition with Event Coincidence Analysis (ECA), referred to as Multi-Scale Event Coincidence Analysis (MSECA) and compare the results with the existing Multi-Scale Event Synchronisation (MSES). From a conceptual perspective, MSECA appears to be a more reasonable method compared to MSES, as it mitigates certain undesired effects of temporal clustering of rainfall extremes across various timescales.

Our results reveal distinct differences in network properties depending on the methodology used, highlighting the sensitivity of network-based analyses to the choice of construction technique. These differences affect the identification of dominant heavy rainfall patterns and their underlying drivers, such as large-scale atmospheric circulation and/or local feedback mechanisms at daily to monthly temporal scales.

Our work underscores the importance of methodological rigor and the potential of complex network approaches in advancing the understanding of extreme rainfall events in monsoon-dominated regions. This comparison provides a foundation for developing standardized practices for network-based climate studies, enabling more robust assessments of extreme weather phenomena.

How to cite: Bishnoi, G., Dhanya, C. T., and Donner, R. V.: A Comparison of Methodologies for Studying Heavy Precipitation Events during the Summer Monsoon Season in India Using Complex Network Approaches, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21222, https://doi.org/10.5194/egusphere-egu25-21222, 2025.

EGU25-292 | ECS | Posters on site | HS3.3

Influence of Temperature on Streamflow Dynamics: A Multi-Catchment Analysis Using the PCMCI+ Causal Discovery Algorithm 

Hossein Abbasizadeh, Petr Maca, and Martin Hanel

While precipitation is the primary driver of streamflow variability, temperature also plays a significant role. Temperature influences streamflow by modifying precipitation, evapotranspiration, and soil moisture. While this relationship is often studied using hydrological or black-box models, the causal effect of temperature dynamics on streamflow at the catchment scale is not fully understood. This study investigates the causal relationship between precipitation, temperature, and streamflow time series using the PCMCI+ causal discovery method. Having the causal structure, the total causal effect of temperature on stream flow is estimated. The analysis is conducted on CAMELS-GB (671 catchments) and LamaH (859 catchments) datasets to study the causal effects of temperature on streamflow across a wide range of catchments with different climate and physiographic characteristics. Preliminary results indicate that temperature significantly influences streamflow within a specific range, which changes over time for most catchments. The changes in the range within which the temperature has high causal effects on the temperature might be due to the shift in catchment storage and precipitation patterns, leading to a change in catchment response to temperature. These findings highlight the importance of identifying a relationship between temperature streamflow variability from a cause-and-effect perspective. This suggests that incorporating causal information can improve the modelling of the hydrological systems under changing climate. 

How to cite: Abbasizadeh, H., Maca, P., and Hanel, M.: Influence of Temperature on Streamflow Dynamics: A Multi-Catchment Analysis Using the PCMCI+ Causal Discovery Algorithm, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-292, https://doi.org/10.5194/egusphere-egu25-292, 2025.

EGU25-482 | ECS | Orals | HS3.3

Equifinality in River Discharge Prediction Revealed Through Explainable AI  

Qiuyang Chen, Simon Mudd, and Simon Moulds

River discharge prediction is critical for water resource management, yet equifinality—where multiple model configurations achieve similar accuracy—complicates process understanding. We explored this phenomenon using Long Short-Term Memory (LSTM) models trained on UK river basins, incorporating geomorphic descriptors derived from Digital Terrain Models and other environmental features from the CAMELS-GB dataset, including land cover, soil, and climate variables. Explainable AI techniques revealed that the models rely on different, yet equally effective, combinations of correlated features to achieve comparable performance. This variability underscores the complexity of hydrological systems and highlights the importance of integrating explainability and domain knowledge in machine learning to enhance model interpretability and robustness.

How to cite: Chen, Q., Mudd, S., and Moulds, S.: Equifinality in River Discharge Prediction Revealed Through Explainable AI , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-482, https://doi.org/10.5194/egusphere-egu25-482, 2025.

EGU25-1863 | ECS | Posters on site | HS3.3

Predicting Water Movement in Unsaturated Soil Using Physics-Informed Deep Operator Networks 

Qiang Ye, Zijie Huang, Qiang Zheng, and Lingzao Zeng

Accurate modeling of soil water movement in the unsaturated zone is essential for effective soil and water resources management. Physics-informed neural networks (PINNs) offer promising potential for this purpose, but necessitate retraining upon changes in initial or boundary conditions, posing a challenge when adapting to variable natural conditions. To address this issue, inspired by the operator learning with more universal applicability than function learning, we develop a physics-informed deep operator network (PI-DeepONet), integrating physical principles and observed data, to simulate soil water movement under variable boundary conditions. In the numerical case, PI-DeepONet achieves the best performance among three modeling strategies when predicting soil moisture dynamics across different testing areas, especially for the extrapolation one. Guided by both data and physical mechanisms, PI-DeepONet demonstrates greater accuracy than HYDRUS in capturing spatio-temporal moisture variations in real-world scenario. Furthermore, PI-DeepONet successfully infers constitutive relationships and reconstructs missing boundary flux condition from limited data by incorporating known prior physical information, providing a unified solution for both forward and inverse problems. This study is the first to develop a PI-DeepONet specifically for modeling real-world soil water movement, highlighting its potential to improve predictive accuracy and reliability in vadose zone modeling by combining data-driven approaches with physical principles.

How to cite: Ye, Q., Huang, Z., Zheng, Q., and Zeng, L.: Predicting Water Movement in Unsaturated Soil Using Physics-Informed Deep Operator Networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1863, https://doi.org/10.5194/egusphere-egu25-1863, 2025.

EGU25-2661 | Posters on site | HS3.3

Using explainable artificial intelligence as a diagnostic tool  

Sheng Ye, Jiyu Li, Yifan Chai, Lin Liu, Murugesu Sivapalan, and Qihua Ran

Recent applications have demonstrated the strength of deep learning (DL) in information extraction and prediction. However, its limitations in interpretability have delayed its popularity for use in facilitating advancement of hydrologic understanding. Here we present a framework using explainable artificial intelligence (XAI) as a diagnostic tool to investigate distributed soil moisture dynamics within a watershed. Soil moisture and its movement generated by physically based hydrologic model were used to train a long short-term memory (LSTM) network, whose feature attribution was then evaluated by XAI methods. The aggregated feature importance presents abrupt rise in the model’s nodes located in riparian area, indicating threshold behavior in runoff generation and development of hydrologic connectivity at the watershed scale, which helps explain the rapid increase in streamflow. This work represents a demonstration of the potential of XAI to uncover underlying physical mechanisms and to help develop new theories from observed data.

How to cite: Ye, S., Li, J., Chai, Y., Liu, L., Sivapalan, M., and Ran, Q.: Using explainable artificial intelligence as a diagnostic tool , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2661, https://doi.org/10.5194/egusphere-egu25-2661, 2025.

EGU25-2740 | ECS | Orals | HS3.3

A General Framework for Integrating Neural Networks into Numerical Resolution Methods for Spatially Distributed Hydrological Models 

Ngo Nghi Truyen Huynh, Pierre-André Garambois, Benjamin Renard, and Jérôme Monnier
Machine learning (ML) methods have been utilized in hydrology for decades. Recently, hybrid approaches that combine data-driven techniques with process-based models have gained attention, highlighting the complementary strengths of ML and physical models. However, the explicability and adaptability of such hybrid models remain open questions. This work introduces a general framework for incorporating neural networks (NNs) and ML techniques into a regionalizable, spatially distributed hydrological model. As a case study, a simple NN is employed to correct internal fluxes within a conceptual GR hydrological model that allows analytical integration. The corresponding hybrid ordinary differential equation set is integrated with an implicit numerical scheme solved by the Newton-Raphson method. Implementation in Fortran-based code supports differentiability, enabling the computation of the cost gradient through a combination of an adjoint model and analytical NN gradients. Results over a large catchment sample show promising improvements in model accuracy and provide insights into hydrological behaviors through interpretable NN outputs. These findings demonstrate the framework's potential to advance hybrid hydrological modeling by enhancing explicability and adaptability. Additionally, the proposed framework offers flexibility for integration into other modeling chains and applications across diverse geophysical models.

How to cite: Huynh, N. N. T., Garambois, P.-A., Renard, B., and Monnier, J.: A General Framework for Integrating Neural Networks into Numerical Resolution Methods for Spatially Distributed Hydrological Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2740, https://doi.org/10.5194/egusphere-egu25-2740, 2025.

EGU25-3859 | ECS | Posters on site | HS3.3

Explainable convolutional neural network for flood susceptibility mapping in Southern Ontario   

Rahma Khalid and Usman T Khan

Flood susceptibility mapping (FSM) plays a crucial role in proactive flood risk management, particularly in light of increasing fluvial flooding events. Traditional FSM methods, such as physics-based and qualitative approaches, are hindered by either high computational demands or inherent uncertainty. To address this, machine learning (ML) models have become an increasingly popular FSM approach, though commonly cited as black-box approaches due to the difficulty associated with understanding their underlying mechanisms. In order to better understand the ML approaches used for FSM, this study uses the gradient-weighted class activation mapping (Grad-CAM) to interpret flood susceptibility predictions of a convolutional neural network (CNN) for the Don River watershed in Ontario, Canada. Grad-CAM is an explainable algorithm highlighting input regions that are influential to the output, aiding the user in understanding and visualizing model selected important features used to arrive at the prediction. Grad-CAM results are compared to the commonly used shapley additive explanation (SHAP) algorithm. SHAP is used to calculate the relative contribution of each input onto the output, and provides a benchmark for comparisons due to its popularity.

A two dimensional CNN with an architecture of two convolutional layers, two pooling layers and a fully connected layer is used to predict flood susceptibility. The inputs to the CNN include topographical and climactic variables across the entire watershed, with a 60-40% training and testing split respectively. The results of the CNN were compared against the floodplain map of the Don River. Using the area under curve- receiver operating characteristics (AUC-ROC) as a performance metric, the CNN exhibits high performance with an AUC-ROC of 0.96.

The study highlights the potential of CNNs for flood susceptibility mapping, as well as compares two explainable machine learning algorithms, helping to further their application within FSM. Explainable algorithms are essential to decision makers in flood risk management for proactive planning and resource allocation. Future work should explore expanding the scope to predict flood susceptibility at a nationwide level.

How to cite: Khalid, R. and Khan, U. T.: Explainable convolutional neural network for flood susceptibility mapping in Southern Ontario  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3859, https://doi.org/10.5194/egusphere-egu25-3859, 2025.

Floods are the costliest hazard in Canada in terms of direct infrastructure damage. Flood susceptibility modelling (FSM) identifies flood hazard areas; input features are dependent on the study area and modelling methods, which affect the reliability and accuracy of FS maps. Typical features in FSM are static topographical inputs (digital elevation model, land use, wetness index, height above nearest drainage, etc.). Though meteorological variables have been included in FSM, they are often low temporal resolution (e.g. annual); seasonal meteorological variables are often not included. The 2023 Canadian National FS map was developed using machine learning (ML) ensembles, with features that include historical flood events and 30 years of climate data. This research initiates the update to the existing Canadian FS map by expanding the suite of input features used and comparing the impact of three feature selection methods (partial correlation, partial mutual information, combined neural pathway strength) on three types of ML algorithms: random forest, artificial neural network (ANN) and convoluted neural network (CNN). The expanded set of features includes geospatial indices and flood-specific meteorological data such as spring temperature, precipitation, and vapour pressure. Data from preceding seasons to specific flood events is also included. Preliminary findings from the feature selection methods show that including seasonal flood-specific meteorological data provides important information leading to better model performance. Model performances of the three algorithms were comparable. Random forest with extreme gradient boosting led to the highest model performance (AUC = 0.98, F1 = 0.94), followed by CNN (AUC = 0.0.96, F1 = 0.90). ANN ensemble with leave-one-out-cross-validation resulted in the lowest model performance (AUC = 0.91, F1 = 0.85). Results contribute to the development of an improved national FS map for Canada.

How to cite: Dunbar, K. E., McGrath, H., and Khan, U. T.: Enhancing flood susceptibility modelling in Canada: Integrating seasonal meteorological data, feature selection and machine learning approaches, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3871, https://doi.org/10.5194/egusphere-egu25-3871, 2025.

EGU25-4428 | ECS | Orals | HS3.3

Towards Physics-consistent Foundation Models for Flood Forecasting 

Qingsong Xu and Xiao Xiang Zhu

Effective flood forecasting is critical for informed decision-making and timely emergency response. Traditional physical models, which rely on fixed-resolution spatial grids and input parameters, often incur substantial computational costs, limiting their capacity to accurately predict flood peaks and provide prompt hazard warnings.  This paper introduces methods to ensure physical consistency in machine learning models, aiming to develop a fast, stable, accurate, cross-regional, and downscaled neural flood forecasting foundation model. Specifically, we present a Physics-embedded Neural Network, which integrates the momentum and mass conservations of flood dynamics into a neural network. Additionally, we combine this Physics-embedded Neural Network with a diffusion-based generative model, enhancing physical process consistency for long-term, large-scale flood forecasting. We also briefly introduce other models that integrate physics and machine learning, such as the FloodCast model by incorporating hydrodynamic equations into its loss function to maintain physical consistency, and the UrbanFloodCast model by learning physical consistency from urban flood dynamic data. The performance of these models will be analyzed using our proposed FloodCastBench dataset, a comprehensive collection of low-fidelity and high-fidelity flood forecasting dataset and benchmark. Results from the dataset demonstrate that incorporating physical consistency significantly enhances flood forecasting accuracy, demystifies the black-box nature of machine learning frameworks, and increases confidence in addressing dynamical systems. Finally, we propose a Spatiotemporal Foundation Model capable of forecasting floods across a variety of scales and regions.

How to cite: Xu, Q. and Zhu, X. X.: Towards Physics-consistent Foundation Models for Flood Forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4428, https://doi.org/10.5194/egusphere-egu25-4428, 2025.

EGU25-4845 | ECS | Posters on site | HS3.3

Using Causal Discovery to Identify Drivers and Controls of Streamflow in Large Sample Hydrology 

David Strahl, Sebastian Gnann, Karoline Wiesner, and Thorsten Wagener

Catchments are the fundamental units of hydrological analysis and integrate a vast number of physical, biological, and anthropogenic processes. Traditional hydrological modelling approaches, however, adopt a bottom-up perspective, aggregating small-scale physical principles to predict large-scale catchment behaviour. While effective for prediction, this approach can fall short in advancing our understanding of emergent processes and their interactions given the strong dependence on a priori assumptions. To address this gap, causal discovery algorithms offer a promising alternative by moving beyond simple correlation to directly identifying the dynamic causal structures emerging at the catchment scale. In this study, we applied the PCMCI+ algorithm to the CAMELS-US dataset in combination with a subsequent causal effect estimation. We explored how and to what extent dynamic causal structures can be learned from hydro-meteorological data alone, and which catchment properties and conditions influence their expression. We find that causal discovery in hydrology faces challenges due to non-stationarity, unsuitable conditional independence tests, and unmet methodological assumptions. Despite these limitations, our approach reconstructed physically plausible relationships controlled by meaningful catchment properties. These results highlight the potential of causal discovery in hydrology, where it could serve as a complementary framework for model evaluation studies or as an integral part of the model development process.

How to cite: Strahl, D., Gnann, S., Wiesner, K., and Wagener, T.: Using Causal Discovery to Identify Drivers and Controls of Streamflow in Large Sample Hydrology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4845, https://doi.org/10.5194/egusphere-egu25-4845, 2025.

EGU25-5052 | ECS | Posters on site | HS3.3

Can CNN-LSTM and lumped models improve (extreme) streamflow prediction of semi-distributed models? A comparative analysis of two hybrid frameworks 

Aseel Mohamed, Awad M. Ali, Ahmed Ali, Osama Hassan, Mohamed E. Elbasheer, and Mutaz Abdelaziz

Water resources management depends heavily on hydrological modeling for reservoir operation and risk mitigation, especially in data-scarce regions. Hybrid approaches that combine artificial intelligence and conceptual models offer great potential for accurate streamflow prediction. However, their implementation can be time-consuming and applied in different configurations. This study comprehensively compares two promising hybrid frameworks: the Conceptual-Data-Driven Approach (CDDA) and the Ensemble Approach. The analysis was conducted in the Upper Blue Nile Basin in Ethiopia over the period from 2002 to 2019. Six baseline models were developed, including CNN-LSTM (data-driven), NAM and HBV-Light (lumped), and SWAT+, WEAP, and HEC-HMS (semi-distributed). All models achieved NSE ≥ 0.85 during the validation period, with CNN-LSTM performing best (NSE = 0.94). Each model was integrated into the two hybrid frameworks using Random Forest (RF) or Artificial Neural Networks (ANN). Results showed that the Ensemble Approach outperformed CDDA by combining two conceptual models. ANN performed better than RF across both frameworks. Hybrid modeling significantly improved semi-distributed models, while lumped and data-driven models showed minimal benefits. In the Ensemble Approach, normal and extreme flows simulated using semi-distributed models performed best when supported by CNN-LSTM or lumped models. Our analysis also demonstrated the robustness of the Ensemble Approach for selecting the supporting model. These findings emphasize the value and feasibility of the Ensemble Approach for improving streamflow prediction and better supporting decision-making in data-scarce regions. Nevertheless, a thorough understanding of the opportunities in hybrid modeling requires further research with a specific focus on operational forecasting.

How to cite: Mohamed, A., M. Ali, A., Ali, A., Hassan, O., E. Elbasheer, M., and Abdelaziz, M.: Can CNN-LSTM and lumped models improve (extreme) streamflow prediction of semi-distributed models? A comparative analysis of two hybrid frameworks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5052, https://doi.org/10.5194/egusphere-egu25-5052, 2025.

EGU25-5727 | ECS | Posters on site | HS3.3

Using Explainable Artifical Intelligence (XAI) to Analyze the Behavior of Global Water Models 

Lea Faber, Karoline Wiesner, Ting Tang, Yoshihide Wada, and Thorsten Wagener

Model Intercomparison Projects in the Earth Sciences have shown, that the outputs of
Earth System Models often show large variations and can therefore give quite different results,
with no single model consistently outperforming others. Examples include Global Water
Models (GWMs), as well as Global Climate Models (GCMs). The high computational costs
of running such models make comprehensive statistical analyses challenging, a common issue
with many complex models today. Machine learning models have become popular surrogates
of slow process-based models, due to their computational speed, at least once trained. This
speed makes it possible to use techniques from Explainable AI (XAI) to analyze the behavior
of the surrogate model.
Here, we analyze long-term averages of the GWM ’Community Water Model’ (CWatM)
for different parts of the global domain for actual evapotranspiration Ea, total runoff Q and
groundwater recharge R. We train an artificial neural network on the model’s input and output
data and use three different strategies to assess the importance of input data: LassoNet for sub-
set selection and feature ranking, along with Sobol’ indices and DeepSHAP for interpretability.
Our results show that subset selection can effectively reduce model complexity before XAI
analysis. For some hydrological domains the number of relevant input
variables for a chosen output reduces to less then 15 variables out of 98 model inputs, while
others remain more complex, requiring many variables for performances with R2 > 0, 8.

How to cite: Faber, L., Wiesner, K., Tang, T., Wada, Y., and Wagener, T.: Using Explainable Artifical Intelligence (XAI) to Analyze the Behavior of Global Water Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5727, https://doi.org/10.5194/egusphere-egu25-5727, 2025.

EGU25-6278 | Orals | HS3.3

Training Surrogates with Knowledge and Data: A Bayesian Hybrid Modelling Strategy 

Anneli Guthke, Philipp Luca Reiser, and Paul Bürkner

Physics-based hydrological modelling provides great opportunities for risk assessment and water resources management. However, diagnostic model evaluation and quantitative uncertainty assessment remain a challenge: (1) Model choices, boundary conditions, and prior assumptions about input, parameter or data uncertainty might be hard to formulate or justify; (2) rigorous propagation of uncertainties struggles when the analysed model structure is not “true”, and (3) a full propagation of uncertainties is often computationally prohibitive for complex models.

Alternative approaches promote the extraction of information directly from data, thereby avoiding overly strict physics-based constraints and the pitfalls of uncertainty quantification. Challenges of these data-driven approaches include the lack (or difficulty of) explainability, transparency, and transferability to unseen scenarios.

To explore the frontier of where those two perspectives (should) converge, we investigate the potential of surrogate models (computationally cheaper, data-driven representations of complex models) as a binding link with several potential benefits: (1) they alleviate the computational burden and thereby allow for a fully Bayesian uncertainty analysis; (2) they are flexible enough to overcome structural deficits of the original complex model, thereby enabling a better predictive performance, and (3) being data-driven, we can elegantly fuse the information from available data into their training process.

Methodologically, we propose a weighted data-integrated training of surrogates via two competing approaches that differ technically, but also philosophically, and reveal complementing insights about the strengths and weaknesses of the physics-based model and about the additional information in the available data, thereby facilitating deeper system understanding and improved (hybrid) modelling. We demonstrate the proposed workflow on didactic examples and a real-world case study. We expect this approach to be generally useful for modelling dynamic systems, as it contributes to more realistic uncertainty assessment and opens up ways for model development.  

How to cite: Guthke, A., Reiser, P. L., and Bürkner, P.: Training Surrogates with Knowledge and Data: A Bayesian Hybrid Modelling Strategy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6278, https://doi.org/10.5194/egusphere-egu25-6278, 2025.

EGU25-7382 | Orals | HS3.3

Dynamical system neural network for hydrological modelling 

Derek Karssenberg

Neural networks are efficient and effective in predicting system states in hydrology. However, most current approaches lack hydrological flow partitioning, do not allow for training on measurements of multiple variables, or lack capability to tightly integrate physically-based components. To address these shortcomings I propose and evaluate an approach referred to below as Dynamical System Neural Network (DSNN). DSNN is a feedforward neural network with an architecture that resembles the organisation in components of the real-world system it represents. In hydrology, the DSNN represents each water flow (e.g. seepage, snow melt) by a collection of input, hidden, and output neural layers, where each input is the state of a hydrological storage (e.g. groundwater storage influencing seepage) or other variable (e.g. air temperature influencing snow melt). These components are interconnected to form a single neural network of the complete dynamical system considered, where all storages and flows are explicitly quantified. If physical understanding of a flow and its parameterization is available, a known formulation can be used as a replacement of a neural network component. The DSNN is applied forward in time, backpropagating gradients over all timesteps. It can be run in spatially lumped or semi-distributed mode. To demonstrate the approach, a DSNN is presented of the Austrian Dorfertal (Kals) Alpine catchment containing snow and subsurface water storages and associated flows including streamflow. The DSNN is trained, validated, and tested on daily streamflow over ~40 years. To explore the capability of the DSNN in estimating the magnitude and dynamics of internal system storages (snow water equivalent, subsurface water storage) and flows (evapotranspiration, sublimation, snowmelt, seepage), the DSNN is first trained and tested with streamflow data generated by a conceptual model. The DSNN turns out to be capable of reproducing - with a satisfactory level of precision - the system states and fluxes calculated by the conceptual model, with decreasing performance when measurement error is added to the artificially generated streamflow data before training. To explore its predictive performance, the DSNN is applied on measured streamflow data for the Dorfertal, comparing multiple DSNN setups that represent all flows as neural network components or only a subset of flows where remaining flows are represented with a standard conceptual model (e.g. linear reservoir). Preliminary results indicate that in predictive performance, in most setups, the DSNN outperforms a standard conceptual model trained on the same streamflow data, with NSE values for testing of 0.74 and 0.71, respectively. This preliminary result indicates DSNN to be a promising approach for blending process-based and neural network based modelling as well as for training (i.e. calibration) of neural network models on measurements of multiple hydrological variables as these are all explicitly represented by the DSNN and can thus be incorporated in the loss function (e.g. streamflow, snow depth, groundwater, evapotranspiration).

How to cite: Karssenberg, D.: Dynamical system neural network for hydrological modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7382, https://doi.org/10.5194/egusphere-egu25-7382, 2025.

EGU25-7770 | Orals | HS3.3

Advancing distributed hydrological modeling with hybrid machinelearning 

Yi Zheng, Chao Wang, and Shijie Jiang
Accurately simulating large-scale water dynamics is important
for managing water resources, addressing climate change impacts, and
understanding hydrological variability. Despite advances in hydrological
modeling, simulating water fluxes and states at global or regional
scales remains challenging due to the complexity of distributed
processes and limited understanding of key components. Encoding physical
knowledge in deep neural networks (NNs) for differentiable modeling
offers a promising solution but has yet to be fully realized for
distributed hydrological models, especially for processes such as river
routing.
This study presents a novel differentiable modeling framework that
bridges physical and data-driven approaches for distributed hydrological
modeling. The framework encodes a large-scale hydrological model (i.e.,
HydroPy) as a neural network, incorporates an additional NN to map
spatially distributed parameters from local climate and land attributes,
and employs NN-based modules to represent poorly understood processes.
Multi-source observations are used to constrain the system in an
end-to-end manner, with the Amazon Basin as a case study to demonstrate
the framework’s applicability and effectiveness.
Results show that the developed model improves simulation accuracy by
30-40% compared to the original hydrological model. Replacing the
Penman-Monteith formulation with NN produces more realistic potential
evapotranspiration estimates. SHAP analysis of the NN parameterization
further reveals how climate and land attributes regulate the spatial
variability of key parameters. Overall, by integrating physical realism
with the flexibility of machine learning, this framework addresses
critical limitations of traditional hydrological models. It provides a
scalable, interpretable approach to advance large-scale hydrological
modeling and address pressing water and climate challenges.

How to cite: Zheng, Y., Wang, C., and Jiang, S.: Advancing distributed hydrological modeling with hybrid machinelearning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7770, https://doi.org/10.5194/egusphere-egu25-7770, 2025.

EGU25-9176 | ECS | Orals | HS3.3

GPU-Enabled Cell-to-Cell Routing in a High Resolution Hybrid Distributed Hydrological Model with Multi-Source Remote Sensing Data Assimilation: A Continental-Scale Computational Approach  

Mouad Ettalbi, Pierre-André Garambois, Ngo-Nghi-Truyen Huynh, Emmanuel Ferreira, and Nicolas Baghdadi

The integration of remote sensing observations into hydrological modeling frameworks presents a significant opportunity for improving spatial and temporal predictive capabilities across continental domains. This research introduces a novel hybrid distributed hydrological model that addresses key challenges in computational efficiency, by using a GPU-enabled computational infrastructure, and in predictive accuracy by assimilating multi-source remote sensing datasets, specifically satellite-based soil moisture and evapotranspiration, at a high spatial resolution (1km×1km) and temporal scale (hourly). The model addresses critical challenges in regional hydrological forecasting by leveraging advanced data assimilation techniques and machine learning methodologies.

The proposed hybrid modeling framework synthesizes physically-based distributed hydrologic modeling principles with data-driven machine learning approaches, facilitating a more comprehensive representation of land surface hydrological processes. A key innovation is the GPU-enabled cell-to-cell routing algorithm, which enables fast and efficient computational processing of complex hydrological connectivity and water movement across large spatial domains. By integrating remote sensing observations, the methodology enables enhanced initial condition specification and improved parameter estimation, particularly in regions characterized by sparse ground-based measurement networks.

Preliminary analytical results demonstrate significant improvements in model performance, particularly in capturing spatial and temporal variability of hydrological states and fluxes. The approach substantively advances current methodological capabilities in hydrological forecasting, offering a promising framework for developping enriched tensorial numerical solvers, addressing complex hydroclimatic prediction challenges in data-limited environments.

How to cite: Ettalbi, M., Garambois, P.-A., Huynh, N.-N.-T., Ferreira, E., and Baghdadi, N.: GPU-Enabled Cell-to-Cell Routing in a High Resolution Hybrid Distributed Hydrological Model with Multi-Source Remote Sensing Data Assimilation: A Continental-Scale Computational Approach , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9176, https://doi.org/10.5194/egusphere-egu25-9176, 2025.

EGU25-10256 | ECS | Orals | HS3.3

Uncovering the Dynamic Drivers of Floods through Interpretable Deep Learning 

Yuanhao Xu and Kairong Lin

The formation of floods, as a complex physical process, exhibits dynamic changes in its driving factors over time and space under climate change. Due to the black-box nature of deep learning, its use alone does not enhance understanding of hydrological processes. The challenge lies in employing deep learning to uncover new knowledge on flood formation mechanism. This study proposes an interpretable framework for deep learning flood modeling that employs interpretability techniques to elucidate the inner workings of a peak-sensitive Informer, revealing the dynamic response of floods to driving factors in 482 watersheds across the United States. Accurate simulation is a prerequisite for interpretability techniques to provide reliable information. The study reveals that comparing the Informer with Transformer and LSTM, the former showed superior performance in peak flood simulation (NSE over 0.6 in 70% of watersheds). By interpreting Informer’s decision-making process, three primary flood-inducing patterns were identified: precipitation, excess soil water, and snowmelt. The controlling effect of dominant factors is regional, and their impact on floods in time steps shows significant differences, challenging the traditional understanding that variables closer to the timing of flood event occurrence have a greater impact. Over 40% of watersheds exhibited shifts in dominant driving factors between 1981-2020, with precipitation-dominated watersheds undergoing more significant changes, corroborating climate change responses. Additionally, the study unveils the interplay and dynamic shifts among variables. These findings suggest that interpretable deep learning, through reverse deduction, transforms data-driven models from merely fitting nonlinear relationships to effective tools for enhancing understanding of hydrological characteristics.

How to cite: Xu, Y. and Lin, K.: Uncovering the Dynamic Drivers of Floods through Interpretable Deep Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10256, https://doi.org/10.5194/egusphere-egu25-10256, 2025.

Earth system data, measured by satellites and terrestrial stations and simulated by increasingly complex models, provide valuable information for identifying functional relationships within the Earth system. These relationships are essential for understanding complex interactions and predicting changes, for example, in climatic or ecological processes, but often only occur in certain spatiotemporal sections or within certain threshold values. With the increasing spatiotemporal resolution of remote sensing products and models, a manual analysis is impractical, and hypothesis-driven approaches can lead to undiscovered hidden relationships. Previous work proposed the SONAR (automated diScovery Of fuNctionAl Relationships) decision-tree algorithm to automatically search for functional relationships in earth system data without a-priori assumptions. We analyzed the proposed algorithm using artificially generated data to evaluate SONAR's functionality.  We tested if the choice of statistical indicator (Pearson’s r, Spearman’s ρ, Kendall’s τ, and Mutual Information) influences the functionality of the SONAR algorithm and which factors are important for the identification of functional relationships. Using 1512 synthetic data sets and the developed SAMPI (Similarity of A Manifested and Prototypical decision tree Indicator) coefficient, we demonstrate how the performance of the algorithm changes under different variations of the data sets - including the number of designated splits, the presence of interfering variables and the strength and nature of the underlying functional relationships. In particular, we show which statistical indicator provides the best results under these conditions. The results demonstrate that the SONAR algorithm is very versatile, especially when employing the most reliable statistical indicator. The SONAR algorithm could, therefore, have far-reaching applications, for example, in analyzing climatic patterns or investigating dependencies between environmental factors.

How to cite: Thöne, C., Bäthge, A., and Reinecke, R.: The effects of different statistical indicators in the new decision-tree-based SONAR algorithm for automated detection of functional relationships in Big Earth Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10444, https://doi.org/10.5194/egusphere-egu25-10444, 2025.

EGU25-11693 | ECS | Posters on site | HS3.3

Universal differential equations for estimating terrestrial evaporation 

Olivier Bonte, Diego G. Miralles, Akash Koppa, and Niko E. C. Verhoest

Terrestrial evaporation (E) is an essential climate variable, linking water, energy and carbon cycles. As E is influenced by the state of the atmospheric boundary layer, vegetation and soil, its modelling is a complex task, resulting in a myriad of simulation approaches. To combine the strong predictive skills of data-driven models with the interpretability and physical consistency of process-based models (PBMs), a new research field of differentiable modelling has emerged1

Here, we present a differentiable framework for E estimation, facilitating online training of NNs as intermediate PBM components. It is inspired by the GLEAM framework for estimating E, which applies offline training (i.e., outside the PBM) of neural networks (NNs) predicting evaporative stress2,3. Building upon the Julia SciML ecosystem’s implementation of universal differential equations4, a wide array of numerical methods are available for solving the PBM’s ordinary differential equations (ODEs) and calculating the parameter sensitivities5. In this way, the effect of the numerical methods on the obtained hybrid model can be investigated, moving beyond the direct automatic differentiation through explicit Euler solutions of ODEs as often applied in other hydrological hybrid modelling approaches. 

 

References

1Shen, C., Appling, A.P., Gentine, P. et al., Differentiable modelling to unify machine learning and physical models for geosciences, Nat. Rev. Earth. Environ., 4, 552–567, 2023, https://doi.org/10.1038/s43017-023-00450-9

2Koppa, A., Rains, D., Hulsman, P. et al., A deep learning-based hybrid model of global terrestrial evaporation, Nat. Commun., 13, 1912, 2022, https://doi.org/10.1038/s41467-022-29543-7

3Miralles, D. G., Bonte, O., Koppa, A. et al., GLEAM4: global land evaporation dataset at 0.1° resolution from 1980 to near present, preprint, 2024, https://doi.org/10.21203/rs.3.rs-5488631/v1 

4Rackauckas, C., Ma, Y.,  Martensen, J. et al., Universal differential equations for scientific machine learning, ArXiv, 2020, https://doi.org/10.48550/arXiv.2001.04385 

5Sapienza, F., Bolibar, J., Schäfer, F. et al., Differentiable Programming for Differential Equations: A Review, ArXiv, 2024, https://doi.org/10.48550/arXiv.2406.09699 

How to cite: Bonte, O., Miralles, D. G., Koppa, A., and Verhoest, N. E. C.: Universal differential equations for estimating terrestrial evaporation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11693, https://doi.org/10.5194/egusphere-egu25-11693, 2025.

EGU25-12068 | ECS | Posters on site | HS3.3

A Physics-Constrained Emulator for High-Resolution Soil Moisture  

Annie Y.-Y. Chang, Elena Leonarduzzi, Christian M. Grams, and Vincent W. Humphrey

Like much of Europe, Switzerland is increasingly experiencing severe summer droughts and heatwaves, prompting the mandate for an advanced national drought monitoring and early warning system. A key component of this initiative is the generation of gridded soil moisture estimates that are spatially distributed, extending beyond measurement stations.  Here, we present the concept of a novel physics-constrained land surface model emulator designed to produce high-resolution (e.g. finer than 250m), gridded soil moisture estimates up to 2m depth across Switzerland's diverse topography and climatic conditions. 

This framework aims to integrate multi-source datasets, including in-situ measurements, and reanalysis products, to train a machine learning based (e.g. Convolutional LSTM, or XGBoost) hybrid emulator that ensures physically consistent outputs. Compared to conventional dynamical land surface models, an emulator has the advantage of being more computationally efficient and less constrained by the specific requirements of a given numerical model (in terms of input variables and technical dependencies). To fulfil the needs of a very diverse user community, ranging from numerical weather prediction to agricultural decision-making, the emulator should be optimized for multi-scale applications, from climatological analysis, to near-real-time monitoring, and to medium-term forecasting.

How to cite: Chang, A. Y.-Y., Leonarduzzi, E., Grams, C. M., and Humphrey, V. W.: A Physics-Constrained Emulator for High-Resolution Soil Moisture , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12068, https://doi.org/10.5194/egusphere-egu25-12068, 2025.

EGU25-12928 | ECS | Orals | HS3.3 | Highlight

Global Vegetation Stress Drivers based on Hybrid Modelling and Explainable AI 

Fangzheng Ruan, Oscar M. Baez-Villanueva, Olivier Bonte, Akash Koppa, Wantong Li, Gustau Camps Valls, Yuting Yang, and Diego G. Miralles

Terrestrial evaporation (E) is a critical component of the water cycle, returning nearly 60% of continental precipitation to the atmosphere and dissipating approximately 50% of surface net radiation. A prevalent approach for estimating E involves computing a theoretical maximum, known as potential evaporation (Ep), and scaling it based on a multiplicative stress factor, often referred to as “evaporative stress” (S) or “transpiration stress” (St) when specifically applied to plant transpiration. Like stomatal or surface conductance, St is governed by a complex nonlinear interplay of environmental drivers such as soil moisture, air temperature, radiation, and atmospheric vapor pressure deficit. This complexity is not yet fully understood, which further hampers its accurate physical modelling and limits our ability to comprehend transpiration’s sensitivity to the changing environment.

The fourth generation of the Global Land Evaporation Amsterdam Model (GLEAM4) has yielded a global dataset of transpiration by integrating multi-source remote sensing data following a hybrid approach, in which Ep is computed based on a process-based model and St is calculated by employing deep neural networks. These neural networks are trained on global eddy covariance and sap flow measurements for both tall and short vegetation, and are informed by a set of environmental controls or biotic factors. These factors include soil moisture, vapor pressure deficit, atmospheric CO2 concentration, wind velocity, air temperature, downwelling shortwave radiation, LAI, and vegetation optical depth. Beyond the predictive capabilities of these deep neural networks, the relationships between environmental controls and St within these neural networks remain under exploration, leaving uncertainty as to whether GLEAM4 accurately represents real-world processes. To explore the relationships, we employ the SHapley Additive exPlanation (SHAP) method, which quantifies the marginal contributions of predictors to model predictions, offering insights into the relative importance of environmental drivers in determining St.

Our findings highlight dominant St drivers across various climatic regimes and ecosystems, revealing their contributions' temporal evolution. Additionally, we investigate how St responds to shifts in environmental conditions, including climate and vegetation changes, water stress, atmospheric aridity, and rising CO2 levels. Our study enhances global understanding of transpiration dynamics and provides critical insights into the impacts of diverse hydroclimatic drivers, thereby supporting broader applications within the hydrology and climate communities.

How to cite: Ruan, F., M. Baez-Villanueva, O., Bonte, O., Koppa, A., Li, W., Camps Valls, G., Yang, Y., and G. Miralles, D.: Global Vegetation Stress Drivers based on Hybrid Modelling and Explainable AI, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12928, https://doi.org/10.5194/egusphere-egu25-12928, 2025.

EGU25-13311 | ECS | Posters on site | HS3.3

Hybrid hydrological modelling of the biophysical impacts of earth’s greening on streamflow 

Georgios Blougouras, Alexander Brenning, Mirco Migliavacca, and Markus Reichstein

Vegetation plays an important but complicated role in modulating land-atmosphere interactions and the water cycle. Under global change, increasing vegetation greenness trends have been observed, which further complicate the control of vegetation in the earth system. Despite growing interest in the role of vegetation in the hydrological processes, large uncertainties still exist, particularly when it comes to the underexplored response of streamflow to vegetation greening. In this study, we explore the watershed-relevant biophysical controls of vegetation greening on streamflow. In order to do so, we develop a hybrid ecohydrological model. This model adheres to the water balance principles, while it simultaneously has a flexible structure that enables integrating physical insights from observational data. The multi-task learning optimization ensures physical consistency across a range of processes and temporal frequencies, which allows us to investigate the cascading impacts of vegetation changes across the water cycle, leading up to the streamflow as an end-process. Ecohydrological insights are directly derived from observational data, while physically meaningful model parameters reflect how ecosystem functions and hydrological processes respond to vegetation changes. We find that the marked change in streamflow can be attributed to vegetation change controls on diverse biophysical processes. Our research highlights the potential of hybrid models to capture complex earth system processes by exploiting multiple observational data streams, machine learning and physical constraints.

How to cite: Blougouras, G., Brenning, A., Migliavacca, M., and Reichstein, M.: Hybrid hydrological modelling of the biophysical impacts of earth’s greening on streamflow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13311, https://doi.org/10.5194/egusphere-egu25-13311, 2025.

Cyanobacterial blooms have become more frequent and intense in Lake Superior since 2012, primarily due to increased nutrient loads, with phosphorus being the main limiting factor. To protect water quality, extensive monitoring of lakes and streams is crucial, but it is not cost-effective or practical to measure nutrients frequently across all ecosystems. This study presents a cost-effective, transferable solution using machine learning (ML) models to predict phosphorus concentrations and loads based on conventional water quality parameters like streamflow, dissolved oxygen, conductivity, turbidity, transparency, and total suspended solids. The research introduces an explainable hybrid ML framework combining probabilistic principal component analysis (P2CA) with several ML models, including Bagging Ensemble Learning, Boosting Ensemble Learning, Gaussian Process Regression, and Support Vector Regression, to enhance prediction accuracy. Results demonstrate that the P2CA-Boosting Ensemble Learning model consistently outperforms other approaches. To confirm its effectiveness, the developed model was tested with the same input data from a different river catchment, proving it works well in different environments. This study highlights the potential of combining P2CA with Boosting Ensemble Learning as a powerful tool for water quality management in streams and rivers.

How to cite: Kumar, A. and Zhang, K.: Development of a hybrid machine learning model to predict total phosphorus in streams over the north shore of Lake Superior, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13799, https://doi.org/10.5194/egusphere-egu25-13799, 2025.

EGU25-15436 | ECS | Orals | HS3.3

The Differentiable Distributed Regression Model (dDRM) Balancing Explainability and Predictive Performance 

Bjarte Beil-Myhre, Rajeev Shrestha, and Bernt Viggo Matheussen

The field of hydrology has undergone significant transformation over the past decade, driven by advancements in machine learning and data-driven techniques. A key breakthrough came from the work of Kratzert et al. (2018), who demonstrated that purely data-driven LSTM models could outperform traditional hydrological models in over 600 catchments across North America. However, while these models significantly improve predictive performance, they often sacrifice interpretability and explainability.

To address this trade-off, researchers have explored new approaches that merge physical principles with data-driven methods. One promising innovation is the concept of differentiable modeling, introduced by Chen et al. in 2022. This approach transforms physical models into differentiable functions, allowing neural networks to represent and learn model parameters. By doing so, differentiable modeling enhances flexibility while maintaining a foundation in physical principles.

This research presents a novel differentiable hydrological model called the Differentiable Distributed Regression Model (dDRM). The dDRM builds on the principles of differentiable modeling with the structure of a conceptually lumped model using a simplified representation of physics ("smooth" HBV model). Inspired by the simplicity of the LSTM model, which aggregates data at the catchment level rather than relying on a grid-based representation, we introduce four equally sized elevation zones instead of grid cells in the dDRM. These zones inherently reflect differences in hydrological processes, such as precipitation, temperature, and snowmelt dynamics, enabling the model to account for spatial heterogeneity while maintaining computational efficiency.

By leveraging the principles of differentiable modeling, the dDRM achieves a balance between explainability and predictive performance. To evaluate model performance, we tested the dDRM across sixty-three catchments in southern Norway, in a gauged setting. Only precipitation and temperature were used as input data. For benchmarking purposes, we also trained an LSTM model to the same catchments. 

Our results demonstrate that the dDRM outperforms the fine-tuned LSTM model in both daily predictions and cumulative runoff volumes. These findings underscore the potential of differentiable hydrological models to bridge the gap between performance and interpretability. By combining physical principles with data-driven techniques, the dDRM provides a pathway toward more effective and understandable forecasting tools in hydrology.

How to cite: Beil-Myhre, B., Shrestha, R., and Matheussen, B. V.: The Differentiable Distributed Regression Model (dDRM) Balancing Explainability and Predictive Performance, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15436, https://doi.org/10.5194/egusphere-egu25-15436, 2025.

Groundwater is a critical resource for drinking water supply, agriculture, and ecosystems in general. In regions facing water scarcity, such as Brandenburg (Germany), effective groundwater management is essential. This requires accurate assessments of groundwater dynamics, which data-driven models can deliver through efficient and reliable groundwater level (GWL) predictions. To effectively develop and apply data-driven models for groundwater level prediction, a deeper understanding of which and how the input features influence the groundwater level prediction is crucial.

Our primary objective is to assess the impact of the input features of a Deep learning (DL) model that predicts GWLs using feature attribution methods. Specifically, the influence of climatic features as well as different land use patterns is examined. This study employs a global DL model based on the Long Short-Term Memory (LSTM) architecture to predict seasonal GWLs for 16 weeks ahead. We utilize a comprehensive set of features, including dynamic features such as climatic variables (e.g., temperature, precipitation, relative humidity) and static features such as Corine land cover. By incorporating these, we aim to capture the complex interactions between climate, landuse and groundwater levels.

For the feature attribution itself, we apply the Shapley value sampling method. It analyses the effect of an alternation of an input feature to the respective chosen objective. The choice of that function is essential for the obtained results. We alternate the corresponding objective function in three distinct ways: first, by using the total change of the predicted GWL for the whole period of interest; second, per prediction horizon, i.e. per predicted week of the 16 week prediction; and third, through a decomposition into partial scale-respective signals of the period of interest using the discrete wavelet transform. Besides understanding which input features are most important for the predictive performance of the LSTM model, the results enable us to identify further aspects of the dynamics learned by the model. For example, if and when the model switches from extrapolation to prediction, and at which temporal scales different factors play a role; e.g. if forest vegetation is more important for seasonal or weekly effects on groundwater levels. This multi-faceted approach allows us to gain a deeper understanding of the factors influencing GWLs and their temporal dynamics, both for static and dynamic input features. Ultimately, feature attribution methods can enhance the awareness for reasonable land-use, hence, groundwater management and lead to better predictive models.

How to cite: Engel, M., Kunz, S., Wetzel, M., and Körner, M.: Multitemporal and Multiscale Feature Attribution Methods to Understand the Impact of Climatic and Land Use Features on the Prediction of Groundwater Levels, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15651, https://doi.org/10.5194/egusphere-egu25-15651, 2025.

The Integrated Multi-satellite Retrievals for GPM (IMERG) is a global satellite-based precipitation dataset that provides near real-time precipitation estimates by combining multiple satellite measurements. IMERG integrates microwave (MW) observations from low-orbit satellites with precipitation estimates inferred from the brightness temperature of geostationary infrared (IR) imagery. MW measurements provide accurate precipitation estimates due to their direct interaction with precipitation particles, while IR measurements offer broader spatial and temporal coverage by inferring precipitation from cloud-top brightness temperatures. Together, these complementary techniques balance precision and coverage to improve global precipitation monitoring. However, IR-based precipitation estimates are inherently less reliable due to the weak direct correlation between brightness temperature and precipitation. Conversely, MW-derived estimates are more accurate but spatially constrained by the limited footprint of low-orbit satellites. To investigate the contributing factors in IR precipitation error calibration, we leveraged ERA5 Land, a high-resolution reanalysis dataset that includes surface variables across nine domains, such as temperature, soil moisture, radiation, and vegetation indices. These variables offer a comprehensive lens for understanding the impact of the land surface on precipitation dynamics. We employed the XGBoost machine learning model to predict the errors in IR precipitation estimates relative to MW-derived benchmarks. Additionally, SHapley Additive exPlanations (SHAP) values were used to interpret the model’s predictions, uncovering how individual input features contribute to error correction.


Our findings indicate that the explainable machine learning model can correct the infrared (IR) precipitation estimates to resemble microwave (MW) products, achieving notable improvements across statistical metrics. In the preliminary analysis of 165 countries and territories, the XGBoost model’s calibration improved the RMSE in all validation datasets, with a median reduction of 19.89% and an average reduction of 22.5%. Similarly, the correlation coefficient improved, with a median increase of 18.43% and an average increase of 54.49%. Moreover, the spatial and temporal distributions of the variables' SHAP values show various patterns. The clustered spatial distribution may represent the local climate attributes in specific geographic regions, providing insights into how regional environmental factors influence precipitation estimates. Meanwhile, the temporal distribution may imply seasonal variation, which can help identify patterns in precipitation dynamics and refine IR-based calibration by accounting for temporal variability in precipitation processes. This study provides a robust framework for leveraging land surface variables to refine IR-based precipitation products. By integrating reanalysis data with machine learning models, we present a scalable solution for improving precipitation monitoring in data-sparse regions, particularly where MW observations are unavailable.

How to cite: Hung, H. T. and Wang, L.-P.: IRMerg: Enhancing Global Infrared Precipitation Estimates with Land Surface Variables and Contributing Factors Analysis Using Explainable Machine Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16863, https://doi.org/10.5194/egusphere-egu25-16863, 2025.

EGU25-16971 | ECS | Orals | HS3.3

The Extrapolation Dilemma in Hydrology: Unveiling the extrapolation properties of data-driven models 

Sanika Baste, Daniel Klotz, Eduardo Espinoza, Andras Bardossy, and Ralf Loritz

Long Short-Term Memory (LSTM) networks have shown strong performance in rainfall–runoff modelling, often surpassing conventional hydrological models in benchmark studies. However, recent studies raise questions about their ability to extrapolate, particularly under extreme conditions that exceed the range of their training data. This study examines the performance of a stand-alone LSTM trained on 196 catchments in Switzerland when subjected to synthetic design precipitation events of increasing intensity and varying duration. The model’s response is compared to that of a hybrid model and evaluated against hydrological process understanding. Our study reiterates that the stand-alone LSTM is characterised by a theoretical prediction limit, and we show that this limit is below the range of the data the model was trained on. We show that saturation of the LSTM cell states alone does not fully account for this characteristic behaviour, as the LSTM does not reach full saturation, particularly for the 1-day events. Instead, its gating mechanisms prevent new information about the current extreme precipitation from being incorporated into the cell states. Adjusting the LSTM architecture, for instance, by increasing the number of hidden states, and/or using a larger, more diverse training dataset can help mitigate the problem. However, these adjustments do not guarantee improved extrapolation performance, and the LSTM continues to predict values below the range of the training data or show hydrologically unfeasible runoff responses during the 1-day design experiments. Despite these shortcomings, our findings highlight the inherent potential of stand-alone LSTMs to capture complex hydro-meteorological relationships. We argue that more robust training strategies and model configurations could address the observed limitations, ensuring the promise of stand-alone LSTMs for rainfall–runoff modelling.

How to cite: Baste, S., Klotz, D., Espinoza, E., Bardossy, A., and Loritz, R.: The Extrapolation Dilemma in Hydrology: Unveiling the extrapolation properties of data-driven models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16971, https://doi.org/10.5194/egusphere-egu25-16971, 2025.

EGU25-18102 | ECS | Posters on site | HS3.3

In the application of physically-based and interpretable AI-based models for streamflow simulation 

Sara Asadi, Patricia Jimeno-Sáez, Adrián López-Ballesteros, and Javier Senent-Aparicio

Precise streamflow forecasting in river systems is crucial for water resources management and flood risk assessment. This study focuses on the Tagus Headwaters River Basin (THRB) in Spain, a key hydrological basin providing essential water for urban, industrial, and irrigation purposes. Additionally, a significant portion of its water resources is transferred to the Segura River Basin through the Tagus-Segura water transfer, Spain’s most extensive hydraulic infrastructure. Given that nearly all available water in the THRB is allocated for these demands, precise streamflow forecasting is vital. For streamflow estimation in this basin, we evaluated the Soil and Water Assessment Tool (SWAT+), a physically-based model, and three AI-based models: support vector regression (SVR), feed-forward neural network (FFNN), and long short-term memory (LSTM) models, across four gauging stations within the THRB. For the AI-based models, rainfall and time-lagged runoff data were used as input data. Additionally, an ensemble machine learning technique was evaluated, using the outputs of both physically-based and AI-based individual models as inputs for the ensemble model. The results show that the AI-based models and the ensemble machine learning technique significantly outperformed the SWAT+ model. While the precision of the AI-based models was considerably higher than that of the SWAT+ model, the application of the ensemble technique enhanced the precision of the AI-based models by 18 to 26% during the calibration period and 4.1 to 9.2% during the validation period. Furthermore, the Shapley Additive Explanations (SHAP) methodology was used to explore how each model contributes to the predictions in the ensemble technique. This work was supported by the Spanish Ministry of Science and Innovation, under grants PID2021-128126OA-I00.

How to cite: Asadi, S., Jimeno-Sáez, P., López-Ballesteros, A., and Senent-Aparicio, J.: In the application of physically-based and interpretable AI-based models for streamflow simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18102, https://doi.org/10.5194/egusphere-egu25-18102, 2025.

EGU25-18468 | ECS | Posters on site | HS3.3

An automated machine learning framework for multi-depth soil moisture prediction using hydro-meteorological datasets 

Vidhi Singh, Abhilash Singh, and Kumar Gaurav

 Soil moisture, one of the essential climate variables, forms a fundamental bridge between hydro-meteorological processes and influence climate dynamics. It is extremely variable and is driven by numerous hydrological, agricultural and ecological factors. Soil moisture subsequently impacts soil forming processes, root zone water availability, infiltration rates, runoff, groundwater storage and vegetation-soil interaction. Despite its significant contribution in hydro-ecological interaction, its variability at subsurface is not yet explored adequately. Precise estimation of soil moisture at various depths is crucial because it affects water retention characteristics and modulates the vertical and lateral movement of water within the soil profile. This subsurface information is integral to understanding recharge rates, groundwater interactions, and the overall water balance within a catchment. In this study, we present an automated machine learning framework designed to predict soil moisture at multiple depths of 10 cm, 20 cm, 30 cm, and 40 cm leveraging Bayesian optimization. We collected data from our hydrological observatory set up constituting an automatic weather station, a pan evaporimeter and a soil moisture recorder. To evaluate model performance, we categorized the dataset into four scenarios (S1, S2, S3, and S4), with each subsequent scenario incorporating a greater number of observations and rainfall events. We used 11 input features to train this AutoML model by integrating several hydrological and meteorological variables with in-situ soil moisture data. Among the predictor variables, humidity, dew point, and rainfall emerged as the most influential factors driving soil moisture variability. The model was trained to calculate the performance metrices for the entire dataset and for subsets containing only rainfall instances. Our optimized model demonstrated superior performance, with an R² of 0.88–0.99 and RMSE < 0.022 for the overall dataset, and R² of 0.76–1.00 with RMSE < 0.06 for rainfall-specific data across all soil moisture depths.

How to cite: Singh, V., Singh, A., and Gaurav, K.: An automated machine learning framework for multi-depth soil moisture prediction using hydro-meteorological datasets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18468, https://doi.org/10.5194/egusphere-egu25-18468, 2025.

EGU25-19057 | ECS | Posters on site | HS3.3

Inference of catchment areas from modeled discharge dynamics 

Fedor Scholz, Christiane Zarfl, Thomas Scholten, and Martin V. Butz

The delineation of catchment areas from elevation is a fundamental step in lumped process-based models (PBMs). Most machine learning (ML) approaches for rainfall-runoff modeling spatially aggregate inputs to represent basin-wide processes. Elevation-based lumping, however, disregards both human interventions such as drainages and underground hydrological flows, which can lead to significant model inaccuracies. In this work, we employ DRRAiNN (Distributed Rainfall-Runoff Artificial Neural Network) – a fully distributed neural network architecture – to infer catchment areas directly from observed precipitation and discharge dynamics without prior delineations.

As a first evaluation of the potential to infer actual catchment areas with DRRAiNN, we trained the model on relatively sparse data from 2006 until 2015: Radolan-based hourly precipitation data as input with a spatial resolution of 4x4 km and only daily discharge measurements from 17 stations in the Neckar river basin as target output. Elevation and solar radition were given as additional parameterization input. As DRRAiNN is fully differentiable, we were then able to infer station-specific attribution maps via backpropagation through space and time. To evaluate the alignment between the inferred attribution maps and elevation-based catchment areas, we compute the Wasserstein distance between attributions inside and outside the catchment boundaries. A higher distance indicates better agreement. The results show that DRRAiNN learns to propagate water in a physically plausible manner. Further, we reveal deviations that indicate additional water flows that are undetectable from elevation data alone. Our findings thus suggest that DRRAiNN captures key rainfall-runoff dynamics while avoiding the limitations of lumped models.

The quantitative evaluations alongside qualitative comparisons underscore the model’s potential for uncovering hidden hydrological processes. We show that catchment area estimates can be inferred from relatively little discharge data, which may, in the future, potentially be substituted by satellite data. As a result, DRRAiNN may be applicable in ungauged catchments. Given actual discharge measurements or discharge estimations, DRRAiNN can be used to analyze the hydrological dynamics of surface and subsurface runoff as well as baseflow esimations and has the potential to uncover unexpected and unknown runoff dynamics that would not be detectable otherwise.

How to cite: Scholz, F., Zarfl, C., Scholten, T., and Butz, M. V.: Inference of catchment areas from modeled discharge dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19057, https://doi.org/10.5194/egusphere-egu25-19057, 2025.

EGU25-20878 | ECS | Orals | HS3.3

High-Resolution Differentiable Models for Operational National and Global Water Modeling and Assessment 

Yalan Song, Chaopeng Shen, Haoyu Ji, and Farshid Rahmani

Continental and global water models have long been trapped in slow growth and inadequate predictive power, as they are not able to effectively assimilate information from big data. While Artificial Intelligence (AI) models greatly improve performance, purely data-driven approaches do not provide strong enough interpretability and generalization. One promising avenue is “differentiable” modeling that seamlessly connects neural networks with physical modules and trains them together to deliver real-world benefits in operational systems. Differentiable modeling (DM) can efficiently learn from big data to reach state-of-the-art accuracy while preserving interpretability and physical constraints, promising superior generalization ability, predictions of untrained intermediate variables, and the potential for knowledge discovery. Here we demonstrate the practical relevance of a high-resolution, multiscale water model for operational continental-scale and global-scale water resources assessment. (https://bit.ly/3NnqDNB). Not only does it achieve significant improvements in streamflow simulation compared to the established national- and global water models, but it also produces much more reliable depictions of interannual changes in large river streamflow, freshwater inputs to estuaries, and groundwater recharge. 

How to cite: Song, Y., Shen, C., Ji, H., and Rahmani, F.: High-Resolution Differentiable Models for Operational National and Global Water Modeling and Assessment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20878, https://doi.org/10.5194/egusphere-egu25-20878, 2025.

EGU25-935 | ECS | Orals | HS3.4

Characterizing possible failure modes: Insights from LSTM-Based Streamflow Predictions 

Sarth Dubey, Pravin Bhasme, and Udit Bhatia

Long Short-Term Memory (LSTM) networks have become popular for streamflow prediction in hydrological systems due to their ability to model sequential data. However, their reliance on lumped catchment representation and climate summaries often limits their capacity to capture spatial heterogeneity in rainfall patterns and evolving rainfall trends, both of which are critical for hydrological consistency. This study explores the limitations of LSTM-based streamflow predictions by employing a distributed conceptual hydrological model, SIMHYD, coupled with Muskingum-Cunge routing, to generate synthetic datasets representing diverse hydroclimatic conditions. These datasets are designed to replicate rainfall-runoff dynamics across selected catchments from all 18 ecoregions in CAMELS-US and key Indian river basins, providing a robust testbed for evaluating model performance under controlled conditions. The pre-trained LSTM model is tested against synthetic discharge data, enabling direct comparisons to assess its ability to simulate realistic hydrological responses. Performance is evaluated using multiple metrics, including Nash-Sutcliffe Efficiency (NSE), Kling-Gupta Efficiency (KGE), Percent Bias (PBIAS), and mean peak timing errors, to identify systematic deviations. Results reveal that LSTM models struggle with spatially variable and temporally shifting rainfall patterns, leading to inaccuracies in peak flow timing, magnitude, and overall discharge volumes. These issues highlight vulnerabilities in current LSTM-based flood forecasting systems, particularly in their ability to generalize across diverse climatic conditions and regions. This study also characterizes specific failure pathways, such as underestimation of extreme events and poor temporal coherence in hydrographs, which are critical for operational forecasting. By diagnosing these limitations, the study provides a framework for integrating process-based hydrological knowledge with data-driven techniques to improve model robustness. The findings underscore the importance of using synthetic datasets and diverse diagnostic tools to evaluate and enhance the reliability of LSTM-based models, paving the way for hybrid approaches capable of addressing the complexities of real-world hydrological systems.

How to cite: Dubey, S., Bhasme, P., and Bhatia, U.: Characterizing possible failure modes: Insights from LSTM-Based Streamflow Predictions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-935, https://doi.org/10.5194/egusphere-egu25-935, 2025.

EGU25-1644 | ECS | Posters on site | HS3.4

Graph-enhanced Neural Operator for Missing Velocities Infilling in River Surface Velocimetry 

Xueqin Chen, Hessel Winsemius, and Riccardo Taormina

Measuring river surface velocity enables river discharge estimation, a fundamental task for hydrologists, environmental scientists, and water resource managers. While traditional image-based velocimetry methods are often effective, they struggle to produce complete velocity fields under complex environmental conditions. Poor lighting, reflective glare, lack of visible surface features, or excessive turbulence can all result in regions where feature tracking fails, leading to gaps in the resolved velocity field. Addressing these gaps through the reconstruction of missing velocity measurements is an important research challenge. Recently, researchers have employed deep learning to address various hydrology problems, demonstrating promising improvements. In this work, we propose a neural operator-based model to address the challenge of missing velocities in river surface velocimetry. Specifically, our model is based on the Fourier neural operator with a graph-enhanced lifting layer. It is trained on the river surface velocimetry reconstruction task using a self-supervised paradigm. Once trained, it can be used to infer missing velocities in unseen samples. Experiments conducted on a dataset collected from a river in the Netherlands demonstrate our approach’s ability to accurately infill missing surface velocities, even when faced with large amounts of missing data. We attribute this robustness to the neural operator’s ability to learn continuous functions, which enhances our model’s capacity for high-level feature representation and extraction. Our findings suggest that the reconstructed velocity fields produced by our model can act as reliable ground truth data for deep learning-based methods. In the future, we aim to improve our model’s performance and generalization by incorporating additional data collected from a wider range of rivers and under varying environmental conditions.

How to cite: Chen, X., Winsemius, H., and Taormina, R.: Graph-enhanced Neural Operator for Missing Velocities Infilling in River Surface Velocimetry, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1644, https://doi.org/10.5194/egusphere-egu25-1644, 2025.

EGU25-2616 | ECS | Posters on site | HS3.4

Dual-Source Adaptive-Fusion Transfer Learning for Hydrological Forecasting in Data-scarce Catchments 

Yuxuan Gao and Dongfang Liang

Historical records observed at hydrological stations are scarce in many regions, bringing significant challenges to the hydrological predictions for these regions. Transfer learning (TL), increasingly applied in hydrology, leverages knowledge from data-rich catchments (sources) to enhance predictions in data-scarce catchments (targets), providing new insight into data-scarce region predictions. Most existing TL approaches pre-train models using large meteoro-hydrological datasets to improve overall generalizability to target catchments. However, the predictive performance for specific catchments would be constrained due to irrelevant source data inputs and the lack of effective source fusion strategies. To address these challenges, this study proposes the Dual-Source Adaptive Fusion TL Network (DSAF-Net), which utilizes a pre-trained dual-branch feature extraction module (DBFE) to extract knowledge from two carefully selected source catchments, minimizing noise and redundancy associated with larger datasets. A cross-attention fusion module is then incorporated to dynamically identify key knowledge of the target catchment and adaptively fuse complementary information. This fusion module is embedded after each layer in the DBFE to enhance multi-level feature integration. Results demonstrate that DSAF-Net achieves superior prediction accuracy to single-source TL and large dataset TL strategies. These findings highlight the potential of DSAF-Net to advance hydrological forecasting and support water resource management in data-scarce regions.

How to cite: Gao, Y. and Liang, D.: Dual-Source Adaptive-Fusion Transfer Learning for Hydrological Forecasting in Data-scarce Catchments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2616, https://doi.org/10.5194/egusphere-egu25-2616, 2025.

EGU25-2761 | ECS | Posters on site | HS3.4

Forecasting Reservoir Inflows Using Regionally Trained and Finetuned LSTM Models: A Case Study with CAMELS-DE 

Gregor Johnen, Andre Niemann, Patrick Nistahl, Alexander Dolich, and Alexander Hutwalker

The increasing frequency of extreme hydrological events, such as floods and droughts, poses significant challenges for operators of drinking water reservoirs in maintaining a balance between water supply and demand. While the security of supply typically requires high water levels to meet consumer demands throughout the year, ensuring flood protection, on the contrary, necessitates that reservoir storage is kept partially free to accommodate high inflows. Accurate inflow forecasting is essential for making risk-based operational decisions, including the timely release of water from drinking water reservoirs to mitigate flood risks. While deep learning approaches, particularly Long Short-Term Memory (LSTM) networks, have become prevalent in rainfall-runoff modeling, most existing studies focus on small, homogeneous datasets limited to single hydrological basins. This study leverages the newly published CAMELS-DE dataset to develop a regionally trained and finetuned LSTM model encompassing 1,582 catchments across Germany. We apply this regional model to five small catchments upstream of drinking water reservoirs and compare its performance against basin-specific LSTM models. Our findings demonstrate that the regionally trained LSTM model significantly improves the accuracy of inflow estimates, especially when finetuned to our target catchments. This is highlighting its potential for enhancing reservoir management strategies in the face of climate change.

How to cite: Johnen, G., Niemann, A., Nistahl, P., Dolich, A., and Hutwalker, A.: Forecasting Reservoir Inflows Using Regionally Trained and Finetuned LSTM Models: A Case Study with CAMELS-DE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2761, https://doi.org/10.5194/egusphere-egu25-2761, 2025.

EGU25-4247 | ECS | Posters on site | HS3.4

From multiple meteorological forecasts to river runoff: Learning and adjusting real-time biases to enhance predictions 

Oliver Konold, Moritz Feigl, Christoph Klingler, and Karsten Schulz

Deep learning models such as the Long Short Term Memory Network (LSTM) are capable of representing rainfall-runoff relationships and outperform classical hydrological models in gauged and ungauged settings (Kratzert et al., 2018). Previous studies have shown that combining multiple precipitation data in a single LSTM significantly improves the accuracy of simulated runoff, as the neural network learns to combine temporal and spatial patterns of inputs (Kratzert et al., 2021). However, every operational runoff forecasting setting requires meteorological forecasts. Nearing et al. (2024) have developed a global runoff forecast model based on an LSTM, with an ECMWF forecasting product as additional input over the forecast horizon. Compared with observed or reanalysis meteorological input data, forecasting products generally have a lower accuracy, with different reliabilities between various forecasting products. This is where the synergies of several meteorological forecasts combined with historical observational and reanalysis data can be used in a single deep learning model.

This study investigates how well LSTMs can predict runoff when trained on (1) multiple archived meteorological forecasts and (2) a combination of multiple archived meteorological forecasts and reanalysis data. All meteorological input data are aggregated to the catchments of the LamaH-CE dataset (Klingler, Schulz and Herrnegger, 2021). Runoff predictions are evaluated for a 24 hours forecasting horizon.  Preliminary analyses indicate that the coupling of reanalysis data and forecasting products from different sources improves the accuracy of operational runoff forecasting, suggesting that the model is able to learn and adjust real-time biases in forecasting data.

 

Klingler, C., Schulz, K. and Herrnegger, M. (2021) ‘LamaH-CE: LArge-SaMple DAta for Hydrology and Environmental Sciences for Central Europe’, Earth System Science Data, 13(9), pp. 4529–4565. DOI: 10.5194/essd-13-4529-2021.

Kratzert, F., Klotz, D., Brenner, C., Schulz, K. and Herrnegger, M. (2018) ‘Rainfall–runoff modelling using Long Short-Term Memory (LSTM) networks’, Hydrology and Earth System Sciences, 22(11), pp. 6005–6022. DOI: 10.5194/hess-22-6005-2018.

Kratzert, F., Klotz, D., Hochreiter, S. and Nearing, G.S. (2021) ‘A note on leveraging synergy in multiple meteorological data sets with deep learning for rainfall–runoff modeling’, Hydrology and Earth System Sciences, 25(5), pp. 2685–2703. DOI: 10.5194/hess-25-2685-2021.

Nearing, G., Cohen, D., Dube, V., Gauch, M., Gilon, O., Harrigan, S., Hassidim, A., Klotz, D., Kratzert, F., Metzger, A., Nevo, S., Pappenberger, F., Prudhomme, C., Shalev, G., Shenzis, S., Tekalign, T.Y., Weitzner, D. and Matias, Y. (2024) ‘Global prediction of extreme floods in ungauged watersheds’, Nature, 627(8004), pp. 559–563. DOI: 10.1038/s41586-024-07145-1.

How to cite: Konold, O., Feigl, M., Klingler, C., and Schulz, K.: From multiple meteorological forecasts to river runoff: Learning and adjusting real-time biases to enhance predictions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4247, https://doi.org/10.5194/egusphere-egu25-4247, 2025.

EGU25-4387 | Orals | HS3.4

Runoff Forecasting in Unmeasured Catchments and Rapid Flash Flood Prediction Based on Deep Learning. 

binlan zhang, qingsong xu, and chaojun ouyang

Runoff forecasting is a long-standing challenge in hydrology, particularly in unmeasured catchments and rapid flash flood prediction. For unmeasured catchment forecasting, we introduce the encoder-decoder-based dual-layer long short-term memory (ED-DLSTM) model[1]. This model fuses static spatial granularity attributes with temporal dynamic variables to achieve streamflow forecasting at a global scale. ED-DLSTM reaches an average Nash efficiency coefficient (NSE) of 0.75 across more than 2000 catchments from historical datasets in the United States, Canada, Central Europe, and the United Kingdom. Additionally, ED-DLSTM is applied to 150 fully ungauged catchments in Chile, achieving a high NSE of 0.65. The interpretability of the transfer capacities of ED-DLSTM is effectively tracked through the cell state induced by adding a spatial attribute encoding module, which can spontaneously form hydrological regionalization effects after performing spatial coding for different catchments.

Moreover, rapid flood prediction with daily resolution is challenged to capture changes in runoff over short periods. To address this, we also propose a benchmark evaluation for runoff and flood forecasting based on deep learning (RF-Bench) at an hourly scale. We introduce the Mamba model to hydrology for the first time. The benchmark also includes Dlinear, LSTM, Transformer, and its improved versions (Informer, Autoformer, Patch Transformer). Results indicate that the Patch Transformer exhibits optimal predictive capability across multiple lead times, while the traditional LSTM model demonstrates stable performance, and the Mamba model strikes a good balance between performance and stability. We reveal the attention patterns of Transformer models in hydrological modeling, finding that attention is time-sensitive and that the attention scores for dynamic variables are higher than those for static attributes.

Our work [2,3] provides the hydrological community with an open-source, scalable platform, contributing to the advancement of deep learning in the field of hydrology.

 

[1] Zhang, B., Ouyang, C., Cui, P., Xu, Q., Wang, D., Zhang, F., Li, Z., Fan, L., Lovati, M., Liu, Y., Zhang, Q., 2024. Deep learning for cross-region streamflow and flood forecasting at a global scale. The Innovation 5, 100617. https://doi.org/10.1016/j.xinn.2024.100617

[2] Zhang, B., Ouyang, C., Wang, D., Wang, F., Xu, Q., 2023. A PANN-Based Grid Downscaling Technology and Its Application in Landslide and Flood Modeling. Remote Sensing 15, 5075. https://doi.org/10.3390/rs15205075

[3] Xu, Q., Shi, Y., Bamber, J.L., Ouyang, C., Zhu, X.X., 2024. Large-scale flood modeling and forecasting with FloodCast. Water Research 264, 122162. https://doi.org/10.1016/j.watres.2024.122162

How to cite: zhang, B., xu, Q., and ouyang, C.: Runoff Forecasting in Unmeasured Catchments and Rapid Flash Flood Prediction Based on Deep Learning., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4387, https://doi.org/10.5194/egusphere-egu25-4387, 2025.

EGU25-4500 | ECS | Posters on site | HS3.4

Leveraging Graph Neural Networks for water level prediction 

George Koutsos, Panagiotis Kossieris, Vasiliki Thomopoulou, and Christos Makropoulos

Accurate water level prediction is essential for flood risk management, water resources management, inland water transportation and climate resilience. Traditional statistical methods, such as autoregressive models, and physically-based hydrological simulations, have been widely used in water level forecasting. However, these approaches often struggle to capture complex, dynamic, and nonlinear interactions in a hydrological system, particularly those affected by climate change. In recent years, machine learning models have emerged as a promising alternative, offering improved predictive accuracy and adaptability across varying environmental conditions. A special type of such models is the Graph Neural Network (GNN), which focuses especially on the reproduction of spatial dependencies, and hence it can be employed to capture the spatial dynamic of the hydrologic/hydraulic system, by treating hydrological networks as graph structures (e.g. nodes as gauges). Going one step further, GNN models can be combined with sequence-based machine learning techniques, such as the Long short-term memory (LSTM) neural network, to capture simultaneously the spatial and temporal dynamics of the system. In this work, we develop and assess a series of advanced hybrid-graph structured machine learning models (such as GNN-LSTM) to make hydrometric predictions across a long river channel. The developed models will be assessed on the basis of alternative performance metrics and against a series of traditional benchmark statistical and machine learning models such as ARIMA and LSTM respectively. As a test case, we exploit data from 19 water level gauges in the Red River of the North, which spans 885 km, serving the natural boundary between North Dakota and Minnesota and has experienced several severe historical flood events.

How to cite: Koutsos, G., Kossieris, P., Thomopoulou, V., and Makropoulos, C.: Leveraging Graph Neural Networks for water level prediction, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4500, https://doi.org/10.5194/egusphere-egu25-4500, 2025.

EGU25-4683 | ECS | Posters on site | HS3.4

Classification-Enhanced LSTM Model for Predicting River Water Levels 

Jiaming Luo

River level predicting underpins the management of water resource projects, steers navigational activities in rivers, and protects the lives and properties of riverside communities, etc. Traditionally, hydrological-hydraulic coupled models have been at the forefront of simulating and predicting river levels, achieving notable success. Despite their utility, these models encounter limitations due to the exhaustive demand for various data types—often difficult to obtain—and the ambiguity in determining downstream boundary conditions for the hydraulic model. Responding to these limitations, this study utilizes Long Short-Term Memory (LSTM) model, a deep learning technique, to predict river levels using upstream discharges. Three approaches were used to further enhance the accuracy and reliability of our model. Firstly, we incorporated historical water level data at or downsteam of the predicted station as input, secondly, we classified the datasets based on physical principles, and thirdly, we employed data augmentation techniques. These methods were evaluated within the Jingjiang-Dongting river-lake system in China. It achieves high prediction accuracy of water level and can mitigate the impact of input inaccuracies. The incorporation of water level data as input and the Classification-Enhanced LSTM model that segregates the input data according to rising and recession trends of water level,significantly improve prediction accuracy under extreme water level conditions compared with other deep learning approaches. The proposed model uses easily accessible data to predict water levels, offering enhanced robustness and new strategies for improving prediction accuracy under extreme conditions. It is applicable for predicting water levels at any hydrological station along a river and can enhance the prediction accuracy of hydraulic models by proving a robust downstream boundary condition.

How to cite: Luo, J.: Classification-Enhanced LSTM Model for Predicting River Water Levels, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4683, https://doi.org/10.5194/egusphere-egu25-4683, 2025.

EGU25-6294 | Orals | HS3.4

Improving generalization of soil moisture prediction using self-supervised learning 

Lijun Wang, Liangsheng Shi, and Shijie Jiang

Accurate soil moisture prediction is increasingly important due to its critical role in water resource management and agricultural sustainability under global climate change. While machine learning models have achieved high accuracy in soil moisture prediction, their ability to generalize to different environmental and meteorological conditions remains a significant challenge. Existing models often perform poorly when applied to conditions that differ from their training data, highlighting the need for approaches that improve generalization while effectively capturing underlying soil moisture dynamics.

In this study, we propose a novel soil moisture prediction model that combines self-supervised learning with a Transformer architecture. The performance of the model was compared with the widely used Long Short-Term Memory (LSTM)-based approach to evaluate its ability to generalize. The proposed model outperformed the baseline in tasks such as capturing extreme soil dryness, adapting to unobserved meteorological humidity conditions, and forecasting soil moisture dynamics at untrained depths. Further analysis revealed that the model’s success stems from its capability to learn comprehensive representations of underlying soil moisture processes. These results highlight the potential of advanced deep learning methods to improve prediction and our process understanding of soil hydrology in a changing climate.

How to cite: Wang, L., Shi, L., and Jiang, S.: Improving generalization of soil moisture prediction using self-supervised learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6294, https://doi.org/10.5194/egusphere-egu25-6294, 2025.

EGU25-7020 | ECS | Posters on site | HS3.4

Improving high-flow forecasting using dynamic multimodal feature fusion 

Konstantina Theodosiadou, Thomas Rodding Kjeldsen, and Andrew Barnes

This study evaluates a new approach to improving streamflow forecasting with deep learning: it focuses on the novel application of a dynamic multimodal feature fusion mechanism that adapts fusion operations based on the data's characteristics. Two baseline Long Short-Term Memory (LSTM) architectures are used, applying two dynamic fusion methods: dynamic operation-level fusion and attention-based fusion, to combine heterogeneous and multisource hydrometeorological data. The models are used for univariate (single flow gauge) and multivariate (multi-gauge) streamflow forecasting approaches. Applying these four approaches to the Severn Basin in the UK, known for long medium- to high-flow periods and shorter low-flow intervals, shows that the dynamic operation-level fusion consistently improved over the attention-based fusion in key performance metrics. In the multivariate case, Nash-Sutcliffe Efficiency (NSE) improved by 1.43%, Mean Absolute Error (MAE) decreased by 1.73%, Mean Absolute Scaled Error (MASE) dropped by 1.82%, and high-peak MAE decreased by 3.36%. For the univariate case, NSE improved by 1.44%, MAE decreased by 4.02%, MASE dropped by 3.89%, and high-peak MAE improved by 2.8%. In addition, multivariate models were considerably faster than univariate models, with training and inference times reduced by 74.57% and 73.81%, respectively. The multivariate models showed a 2.75% increase in NSE and a 72.04% decrease in MASE, indicating they captured better the hydrologic variability than the univariate models. Conversely, univariate models had a 20.59% lower MAE, a 21.17% lower high-peak MAE, and greater stability as indicated by tighter interquartile ranges, suggesting better error minimisation and more reliable predictions. Notably, in two river stations all models underperformed due to rapid flow variability and flashy hydrological responses in smaller catchment areas, suggesting in the future the use of higher-resolution climatic data. Overall, the study shows the potential of new dynamic multimodal fusion techniques, navigating the operational trade-offs between speed, stability, and accuracy across multi and uni-variate training strategies in streamflow forecasting. Nonetheless, the need for an optimal operational balance remains, suggesting further refinement of fusion techniques and focusing on minimising uncertainty.

How to cite: Theodosiadou, K., Rodding Kjeldsen, T., and Barnes, A.: Improving high-flow forecasting using dynamic multimodal feature fusion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7020, https://doi.org/10.5194/egusphere-egu25-7020, 2025.

EGU25-7094 | ECS | Posters on site | HS3.4

Enhancing River Nutrient Predictions with Extreme Weather Indices and DL-Physical Hybrid Structures for Improved Interpretability 

Jiayi Tang, Leyang Liu, Kwok Chun, and Ana Mijic

Accurate nutrient predictions are crucial for river water quality management. While deep learning (DL) has shown promise in various Earth science applications, challenges such as data scarcity and limited interpretability hinder its use in river nutrient predictions. Building on insights into the physical dynamics of nutrients, this research investigates how incorporating extreme weather indices as additional input data, which are often overlooked in current DL-based nutrient prediction, could affect model performance. Additionally, we aim to improve model interpretability by developing hybrid DL-physical structures and identify the optimal structure for predicting nutrient indicators. 
 
The study proposes an assessment workflow and demonstrates its application by predicting dissolved inorganic nitrogen (DIN) and soluble reactive phosphorus (SRP) concentrations at the outlet of the Salmons Brook catchment, UK, where nutrient observations are scarce. The workflow includes two key decisions: selecting the input dataset and defining the DL-physical hybrid structure, each with two options. Comparing multiple predictions generated from all decision combinations enables the evaluation of the impacts of extreme weather events and different hybrid structures. 
 
The simulations demonstrate that incorporating extreme weather indices as additional inputs enhanced performance for both nutrient indicators, particularly in capturing extreme values. Overall, the choice of input dataset had a greater impact on the simulations than the hybrid structure, highlighting the importance of careful input selection and preprocessing in DL model development. Integrating results from a physical model into a DL model can improve simulation interpretability by introducing nutrient-related physical processes. In addition to the hybrid structure, incorporating insights into the physical behaviour of nutrients further enhances the interpretability of DL-based predictions, which is crucial for gaining the trust of domain experts, especially when validating results. 

How to cite: Tang, J., Liu, L., Chun, K., and Mijic, A.: Enhancing River Nutrient Predictions with Extreme Weather Indices and DL-Physical Hybrid Structures for Improved Interpretability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7094, https://doi.org/10.5194/egusphere-egu25-7094, 2025.

EGU25-7205 | ECS | Orals | HS3.4

Evaluating uncertainty in probabilistic deep learning models using Information Theory 

Manuel Alvarez Chaves, Hoshin Gupta, Uwe Ehret, and Anneli Guthke

Deep learning methods in hydrology have traditionally focused on deterministic models, limiting their ability to quantify prediction uncertainty. Recent advances in generative modeling have opened new possibilities for probabilistic modelling in various applied fields, including hydrological forecasting (Jahangir & Quilty, 2024). These models learn to represent underlying probability distributions using neural networks, enabling uncertainty quantification through sampling in a very flexible framework.

In this submission we introduce vLSTM, a variational extension of the traditional long short-term memory (LSTM) architecture that quantifies predictive uncertainty by adding noise sampled from a learned multivariate Gaussian distribution to perturb the model’s hidden state. The vLSTM preserves the traditional LSTM’s state-space dynamics while introducing a probabilistic component that enables uncertainty quantification through sampling. Unlike mixed-density networks (MDNs) which directly model the distribution of the target variable, vLSTM’s uncertainty is obtained by perturbations to the hidden state, providing a novel approach to probabilistic prediction. In rainfall-runoff modeling, vLSTM offers a different mechanism for uncertainty quantification to the well established MDN models (Klotz et al., 2022). This approach enriches the existing toolkit of uncertainty methods in deep learning while maintaining the simplicity of sampling for probabilistic predictions.

To rigorously evaluate probabilistic predictions across different model architectures, we develop new information-theoretic metrics that capture key aspects of how uncertainty is handled by a particular model. These include the average prediction entropy H(X), which quantifies model confidence, and average relative entropy DKL(pq), which measures the average alignment between the predicted distribution of a model and a target, among others. The proposed metrics take advantage of non-parametric estimators for Information Theory which have been implemented in the easy to use UNITE toolbox (https://github.com/manuel-alvarez-chaves/unite_toolbox). By expressing these metrics in compatible units of bits (or nats), we enable direct comparisons between different uncertainty measures. We apply these metrics to our newly introduced vLSTM and the existing MDN models to show strengths and weaknesses of each approach. This information-theoretic framework provides a unified language for analyzing and understanding predictive uncertainty in probabilistic models.

References

  • Jahangir, M. S., & Quilty, J. (2024). Generative deep learning for probabilistic streamflow forecasting: Conditional variational auto-encoder. Journal of Hydrology, 629, 130498. https://doi.org/10.1016/j.jhydrol.2023.130498
  • Klotz, D., Kratzert, F., Gauch, M., Keefe Sampson, A., Brandstetter, J., Klambauer, G., Hochreiter, S., & Nearing, G. (2022). Uncertainty estimation with deep learning for rainfall–runoff modeling. Hydrology and Earth System Sciences, 26(6), 1673–1693. https://doi.org/10.5194/hess-26-1673-2022

How to cite: Alvarez Chaves, M., Gupta, H., Ehret, U., and Guthke, A.: Evaluating uncertainty in probabilistic deep learning models using Information Theory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7205, https://doi.org/10.5194/egusphere-egu25-7205, 2025.

EGU25-7468 | ECS | Posters on site | HS3.4

Empirical Evidence of the Importance of Data Recency in LSTM-Based Rainfall-Runoff Modeling  

Qiutong Yu and Bryan Tolson

Deep learning (DL)-based hydrological models, particularly those using Long Short-Term Memory (LSTM) networks, typically require large datasets for effective training. In the context of large-scale rainfall-runoff modeling, dataset size can refer to either the number of watersheds or the length of the training period. While it is well established that training a regional model across more watersheds improves performance (Kratzert et al., 2024), the benefits of extending the training period are less clear.

Empirical evidence from studies such as Boulmaiz et al. (2020) and Gauch et al. (2021) suggests that longer training periods enhance LSTM performance in rainfall-runoff modeling. This improvement is attributed to the need for extensive datasets to ensure proper model convergence and the ability to capture a wide range of hydrological conditions and events. However, these studies neglected the influence of data recency (or data recentness), which is critical for operational applications that forecast current and future hydrological conditions. In the context of climate change and anthropogenic interventions, the assumption of stationarity (i.e., that historical patterns reliably represent future conditions) may no longer hold for hydrological systems (Shen et al., 2022). Consequently, the selection of training periods should account for potential non-stationarity, as more recent data may better reflect current rainfall-runoff dynamics. Intriguingly, Shen et al. (2022) found that calibrating hydrologic models to the latest data is a superior approach compared to using old data, and completely discarding the oldest data can even improve the performance in streamflow prediction.

This study aims to address two research questions: (1) As the number of watersheds increases, is it still necessary to train LSTM models on decades of historical observations? (2) Can LSTM models achieve comparable performance using shorter training periods focused on more recent data? Specifically, we examine whether models trained on recent data outperform those trained on older data and explore how different temporal partitions of historical records affect predictive skill.

This study leverages a comprehensive dataset comprising streamflow records from over 1,300 watersheds across North America, representing diverse climatic and hydrological regimes, with streamflow data spanning 1950 to 2023. Training periods are designed to isolate the effects of temporal data recency while keeping period lengths consistent. This approach enables a systematic comparison of model performance using exclusively older (e.g., pre-1980) versus exclusively recent data (e.g., post-1980). This research provides evidence-based recommendations for selecting training data while balancing computational costs, data availability, and prediction accuracy.

 

References

Boulmaiz, T., Guermoui, M., and Boutaghane, H.: Impact of training data size on the LSTM performances for rainfall–runoff modeling, Model Earth Syst Environ, 6, 2153–2164, https://doi.org/10.1007/S40808-020-00830-W/FIGURES/9, 2020.

Gauch, M., Mai, J., and Lin, J.: The proper care and feeding of CAMELS: How limited training data affects streamflow prediction, Environmental Modelling and Software, 135, https://doi.org/10.1016/j.envsoft.2020.104926, 2021.

Kratzert, F., Gauch, M., Klotz, D., and Nearing, G.: HESS Opinions: Never train an LSTM on a single basin, Hydrology and Earth System Science, https://doi.org/10.5194/hess-2023-275, 2024.

Shen, H., Tolson, B. A., and Mai, J.: Time to Update the Split-Sample Approach in Hydrological Model Calibration, Water Resour Res, 58, e2021WR031523, https://doi.org/10.1029/2021WR031523, 2022.

How to cite: Yu, Q. and Tolson, B.: Empirical Evidence of the Importance of Data Recency in LSTM-Based Rainfall-Runoff Modeling , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7468, https://doi.org/10.5194/egusphere-egu25-7468, 2025.

EGU25-7531 | ECS | Orals | HS3.4

Predicting total organic carbon loads in river using a mass-conserving LSTM integrated with QUAL2E kinetics 

Hyemin Jeong, Byeongwon Lee, Younghun Lee, and Sangchul Lee

The increasing complexity of water pollution and its impact on aquatic ecosystems necessitates the accurate prediction of water pollutant loads for effective river management. Total Organic Carbon (TOC), a key indicator of organic pollution levels, is central to assessing ecosystem health and informing water treatment strategies. However, conventional process-based modeling methods, while capable of providing precise water quality predictions, require extensive input data and significant computational resources, limiting their practical application. Consequently, alternative modeling approaches, particularly those leveraging artificial intelligence, have been explored. Recent advancements in deep learning have improved predictive modeling in environmental sciences. These approaches have showed effectiveness in hydrological applications, such as streamflow forecasting, by capturing complex nonlinear relationships within environmental systems. Despite these advancements, a notable limitation of these models is their difficulty in maintaining physical consistency, specifically in adhering to the principle of mass balance—a fundamental concept in both hydrology and water quality modeling. In this study, we evaluate a Mass-Conserving Long Short-Term Memory network integrated with QUAL2E kinetics (MC-LSTM-QUAL2E) to predict TOC loads in river systems. By incorporating representations of decay and reaeration processes within a mass-conserving neural network framework, this model combines data-driven prediction capabilities with the requirements of physical consistency. A key component of this framework is the trash cell, designed to simulate TOC transformations based on QUAL2E dynamics. Within the trash cell, TOC decay and reaeration are modeled using parameters kdecay​ and kreaeration​, which are determined by environmental variables such as temperature, pH, dissolved oxygen, total nitrogen, and total phosphorus. The QUAL2E module updates the trash state at each timestep to account for TOC losses due to decay and gains from reaeration, ensuring mass conservation.  The MC-LSTM-QUAL2E model was compared to a conventional LSTM model using environmental variables, including temperature, pH, dissolved oxygen, and nutrient levels, as inputs. The analysis used data from 2012 to 2020, with the period from 2012 to 2017 designated for training and 2018 to 2020 for tests. Model performance was assessed using metrics such as Nash-Sutcliffe Efficiency (NSE), Kling-Gupta Efficiency (KGE), Root Mean Square Error-observations standard deviation Ratio (RSR), and Percent Bias (PBIAS). By maintaining mass balance and incorporating QUAL2E dynamics, the model provides reliable predictions of TOC loads in river systems and offers insights into associated biochemical and hydrological processes.

How to cite: Jeong, H., Lee, B., Lee, Y., and Lee, S.: Predicting total organic carbon loads in river using a mass-conserving LSTM integrated with QUAL2E kinetics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7531, https://doi.org/10.5194/egusphere-egu25-7531, 2025.

EGU25-8045 | Posters on site | HS3.4

Developing a Deep Learning-Based Super-Resolution Urban Flood Model: Towards Scalable and Reliable Hydrological Predictions 

Hyeonjin Choi, Hyuna Woo, Minyoung Kim, Hyungon Ryu, Junhak Lee, Seungsoo Lee, and Seong Jin Noh

Integrating deep learning techniques into hydrology has opened a new way to improve urban flood modeling, with various solutions being developed to address urban flood problems driven by climate change and urbanization. However, predicting urban inundation in near real-time for large urban areas remains challenging due to computational demands and limited data availability. This work proposes a deep learning-based super-resolution framework that enhances the spatial resolution of process-based urban flood modeling outputs using convolutional neural networks (CNNs) while improving computational efficiency. This study investigates the interaction between deep learning model architecture and the underlying physical processes to improve prediction accuracy and robustness in urban pluvial flood mapping. The methodology will be applied to various urban flood scenarios, including extreme rainfall events and hurricane-induced flooding, and its performance will be evaluated through quantitative indicators and sensitivity analyses. The applicability and scalability of this model will also be discussed. In particular, strategies to enhance model reliability and integrate additional hydrological information under extreme conditions will be explored. The study will further address uncertainty estimation in deep learning-based super-resolution models and scalability challenges associated with super-resolution approaches for large-scale flood simulations. The findings aim to demonstrate the potential of deep learning as an innovative tool in hydrological modeling and to enable more effective flood risk management strategies.

How to cite: Choi, H., Woo, H., Kim, M., Ryu, H., Lee, J., Lee, S., and Noh, S. J.: Developing a Deep Learning-Based Super-Resolution Urban Flood Model: Towards Scalable and Reliable Hydrological Predictions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8045, https://doi.org/10.5194/egusphere-egu25-8045, 2025.

EGU25-9088 | ECS | Orals | HS3.4

Projecting storm surge extremes with a deep learning surrogate model 

Emiliano Longo, Andrea Ficchì, Sanne Muis, Martin Verlaan, and Andrea Castelletti

Sea level rise and increasing coastal flood risks demand the development of accurate and efficient coastal risk models capable of generating large ensembles of projections to support robust adaptation strategies. The latest IPCC report emphasizes the importance of projecting storm surge changes and their associated uncertainties, alongside mean sea level rise. However, the high computational cost of storm surge simulations continues to limit the feasibility of generating large ensembles.
Artificial Intelligence (AI) is emerging as a promising alternative to simulate storm surge scenarios with significantly reduced computational costs. Despite recent advancements, key challenges remain in accurately representing extreme events and ensuring robust model extrapolation under changing climate conditions. While AI-based surrogate models have been proposed in the literature, gaps persist in understanding their performance limits for extreme events in future scenarios, hindering their application in climate adaptation planning.
To address these challenges, we developed a deep learning (DL) surrogate model of the physics-based Global Tide and Surge Model (GTSM). The DL model is trained using reanalysis data (ERA5) and historical scenarios from the Coupled Model Intercomparison Project Phase 6 (CMIP6) High Resolution Model Intercomparison Project (HighResMIP). Our analysis focuses on the DL model's performance in simulating extreme storm surge events, validated against GTSM outputs for both historical reanalysis and future projections, with a case study along the New York coastline.
To enhance the surrogate model’s performance for extreme events, we explore various loss functions, including a customized quantile loss function, and test alternative DL architectures with different input configurations. Results demonstrate that the quantile loss improves the model's accuracy for extremes compared to standard loss functions such as mean square error. Additionally, fine-tuning DL models with specific Global Climate Model forcing fields improves the alignment of AI-predicted storm surge trajectories with GTSM outputs, even under diverse spatiotemporal resolutions and model setups.
These findings highlight the critical importance of selecting appropriate loss functions and training datasets to ensure robust performance over extreme events and projected future scenarios. Our globally applicable framework, relying solely on open-source data, offers a promising pathway to scalable and efficient storm surge projections, with implications for robust coastal adaptation planning.

How to cite: Longo, E., Ficchì, A., Muis, S., Verlaan, M., and Castelletti, A.: Projecting storm surge extremes with a deep learning surrogate model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9088, https://doi.org/10.5194/egusphere-egu25-9088, 2025.

EGU25-10650 | ECS | Posters on site | HS3.4

The relationship between theoretical maximum prediction limits of the LSTM and network size 

Daniel Klotz, Sanika Baste, Ralf Loritz, Martin Gauch, and Frederik Kratzert

Machine learning is increasingly important for rainfall–runoff modelling. In particular, the community started to widely adopt the Long Short-Term Memory (LSTM) network. One of the most important established best practices  in this context is to train the LSTMs on a large number of diverse basins  (Kratzert et al., 2019; 2024). Intuitively, the reason for adopting this practice is that training deep learning models on small and homogeneous data sets (e.g., data from only a single hydrological basin) leads to poor generalization behavior — especially for high-flows. 

 

To examine this behavior, Kratzert et al. (2024) use a theoretical maximum prediction limit for LSTMs. This theoretical limit is computed as the L1 norm (i.e., the sum of the absolute values of each vector component) of the learned weight vector that relates the hidden states to the estimated streamflow. Hence, for random vectors we could simply obtain larger theoretical limits by increasing the size of the network (i.e., the  number of parameters). However, since LSTMs are trained using gradient descent, this relationship is more intricate. 

 

This contribution explores the relationship between the theoretical limit and the network size. In particular, we will look at how increasing the network size in untrained models increases the prediction limit and contrast it to the scaling behavior of trained models.



How to cite: Klotz, D., Baste, S., Loritz, R., Gauch, M., and Kratzert, F.: The relationship between theoretical maximum prediction limits of the LSTM and network size, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10650, https://doi.org/10.5194/egusphere-egu25-10650, 2025.

EGU25-11240 | ECS | Orals | HS3.4

Exploring the Transferability of Knowledge In Deep Learning-Based Streamflow Models Across Global Catchments 

Jamal Hassan, John Rowan, and Nandan Mukherjee

Accurate streamflow prediction is critical for flood forecasting and water resource management, particularly in data-scarce regions like Central Asia (CA), where traditional hydrological models struggle due to insufficient discharge data. Deep learning models, such as Long Short-Term Memory (LSTM), have demonstrated the potential for global hydrologic regionalization by leveraging both climate data and catchment characteristics. We used a transfer learning (TL) approach to improve streamflow predictions by first pretraining LSTM models on catchments from data-rich regions like Switzerland, Scotland, and British Columbia (source regions). These deep learning models were then fine-tuned on the data scarce target region (CA basins). This approach leverages the knowledge gained from the source regions to adapt the model to the target region, enhancing prediction accuracy despite the data scarcity in CA. Incorporating lagged streamflow alongside ERA-5 climate data boosted prediction accuracy, particularly in snowmelt and glaciers influenced basins like Switzerland (median NSE=0.707 to 0.837), British Columbia (median NSE= 0.775 to 0.923) and CA (median NSE=0.693 to 0.798). K-Means algorithm was applied to categorize catchments from four global locations into five clusters (labeled 0–4) based on their specific attributes. The predictive performance of fine-tuned LSTM model has significantly enhanced when leveraging a pre-trained model with cluster 2, as demonstrated by higher median metrics (NSE=0.958, KGE=0.905, RMSE=10.723, MSE=115.055) compared to both the locally trained model (NSE=0.851, KGE=0.792, RMSE=20.377, MSE=415.579) and individual basin-based training approaches (NSE=0.69, KGE=0.692, RMSE=25.563, MSE=676.110). These results highlight the effectiveness of pretraining the LSTM model on diverse clusters (0, 1, 2, and 4) before fine-tuning on the target region (cluster 3). Moreover, pretraining the LSTM model with clusters 0 and 4 resulted in enhanced performance by increasing the number of basins, whereas the impact was minimal or even declined when using clusters 1 and 2, as well as when all basins from the four clusters were included. These findings demonstrate the feasibility of transfer learning in addressing data scarcity challenges and underscore the importance of diverse and high-quality training data in developing robust, regionalized hydrological models. This approach bridges the gap between data-rich and data-scarce regions, offering a pathway to improved flood prediction and water resource management.

How to cite: Hassan, J., Rowan, J., and Mukherjee, N.: Exploring the Transferability of Knowledge In Deep Learning-Based Streamflow Models Across Global Catchments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11240, https://doi.org/10.5194/egusphere-egu25-11240, 2025.

EGU25-11682 | ECS | Posters on site | HS3.4

Improving AI-based discharge forecasting through hydrograph decomposition and data assimilation 

Bob E Saint Fleur, Eric Gaume, and Nicolas Akil

Effective discharge forecasting is critical in operational hydrology. This study explores novel methods to improve forecast accuracy by combining data assimilation techniques and hydrograph decomposition. Traditional rainfall-runoff modeling, including AI-based approaches, typically simulates the entire discharge signal using a single model. However, runoff is generated by multiple processes with contrasting kinetics, which a single-model approach may fail to capture adequately. This study proposes using hydrograph decomposition to separate baseflow and quickflow components, training specific forecasting models for each component individually, and then merging their outputs to reconstruct the total discharge signal. This approach is expected to enhance forecast accuracy for both floods and droughts, identifying long-term dependencies governing baseflow to improve seasonal low-flow forecasts. Experiments will be conducted using a subset of the CAMELS dataset.

How to cite: Saint Fleur, B. E., Gaume, E., and Akil, N.: Improving AI-based discharge forecasting through hydrograph decomposition and data assimilation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11682, https://doi.org/10.5194/egusphere-egu25-11682, 2025.

EGU25-12110 | Orals | HS3.4

Increasing the Accuracy and Resilience of Streamflow Forecasts through Data Augmentation and High Resolution Weather Inputs 

David Lambl, Simon Topp, Phil Butcher, Mostafa Elkurdy, Laura Reed, and Alden K. Sampson

Accurately forecasting streamflow is essential for effectively managing water resources. High-quality operational forecasts allow us to prepare for extreme weather events, optimize hydropower generation, and minimize the impact of human development on the natural environment. However, streamflow forecasts are inherently limited by the quality and availability of upstream weather sources. The weather forecasts that drive hydrological modeling vary in their temporal resolutions and are prone to outages, such as the ECMWF data outage in November of 2023. 

Here, we present HydroForecast Short Term 3 (ST-3), a state-of-the-art probabilistic deep learning model for medium-term (10-day) streamflow forecasts. ST-3 combines long short-term memory architecture with Boolean tensors representing data availability and dense embeddings for processing of the information in these tensors. This architecture allows for a training routine that implements data augmentation to synthesize varying amounts of availability of weather inputs. The result is a model that 1) makes accurate forecasts even in the case of an upstream data outage, 2) achieves higher accuracy by leveraging data of varying temporal resolutions including regional weather inputs with shorter lead times than the most common medium term weather inputs, and 3) generates individual forecast traces for each individual weather source, facilitating inference across regions where weather data availability is limited. 

Initial results across CAMELS sites in North America indicate that the incorporation of near-term high resolution weather data increases early horizon forecast KGE by nearly 0.25 with meaningful improvements in metrics seen across our customers’ operational sites. Validation metrics across individual weather sources, as well as model interrogation through integrated gradients highlights a high level of fidelity in the model’s learned physical relationships across forecast scenarios.

How to cite: Lambl, D., Topp, S., Butcher, P., Elkurdy, M., Reed, L., and Sampson, A. K.: Increasing the Accuracy and Resilience of Streamflow Forecasts through Data Augmentation and High Resolution Weather Inputs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12110, https://doi.org/10.5194/egusphere-egu25-12110, 2025.

Machine learning (ML) models have transformed our ability to perform reasonably-accurate, large-scale river discharge modeling, opening new opportunities for global prediction in ungauged basins. These ML models are data-hungry, and results have conclusively shown that ML techniques do best when a single ML model is trained on all basins in the dataset. This is contrary to inuitions from the hydrological sciences, where individual basin calibration traditionally provides the best forecasts. 

 

We bridge this gap between intuitions from traditional ML and hydrology by pre-training a single global model on basins in the worldwide Caravan dataset (~6000 basins), and then fine-tune that model on individual basins. This is a well-known practice within ML, and for us serves the purpose of producing models aimed at high-quality local prediction problems while still capturing the advantages of large-sample training. We show that this leads to a significant skill improvement. 

 

We have also conducted analysis of geophysical and hydrological regimes that benefit most from fine-tuning. These results point to how flood forecasting and water management agencies and operators can expect to fine-tune large, pretrained models on their own local data, which may be proprietary and not part of large, global training datasets.

 

This work illustrates how local agencies like national hydromet agencies or flood forecasting agencies might be able to leverage machine learning based hydrological forecast models while also maximizing the value and information of local data by tailoring large, pretrained models to their own local context. This is an important step in allowing local agencies to take ownership of these global models, and directly incorporate local hydrological understanding to improve performance.

How to cite: Ryd, E. and Nearing, G.: Fine Flood Forecasts: Calibrating global machine learning flood forecast models at the basin level through fine-tuning., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13027, https://doi.org/10.5194/egusphere-egu25-13027, 2025.

EGU25-13844 | ECS | Orals | HS3.4

AIFAS: Probabilistic Global River Discharge Forecasting 

Mohamad Hakam Shams Eddin, Yikui Zhang, Stefan Kollet, and Juergen Gall

Hydrological models are vital in river discharge to issue timely flood warnings and mitigate hydrological risks. Recently, advanced techniques in deep learning have significantly enhanced flood prediction by improving the accuracy and efficiency of forecasts, enabling more reliable early warnings and decision-making in flood risk management. Nevertheless, current applications of deep learning methods are still more restricted to local-scale models or in the best case on selected river points at a global scale. Many studies also lack spatial and topological information for training deep learning models, which can limit their generalization ability when applied to large regions with heterogeneous hydrological conditions. In addition, the lack of probabilistic forecasting impedes the quantification of uncertainty in flood predictions. Here we present the Artificial Intelligence Flood Awareness System (AIFAS) for probabilistic global river discharge forecasting. AIFAS is a generative AI model that is trained with long-term historical reanalysis data and can provide grid-based global river discharge forecasting at 0.05°. At the core of our model are the built-in vision module upon state space model (SSM) [1] and the diffusion-based loss function [2]. The vision SSM allows the model to connect the routing of the channel networks globally, while the diffusion loss generates ensembles of stochastic river discharge forecasts. We evaluate the AIFAS forecast skill against other state-of-the-art deep learning models, such as Google LSTM [3], climatology baseline, persistence baseline, and operational GloFAS forecasts [4]. The impact of different hydrometeorological products that drive AIFAS performance on different forecasting lead times will also be discussed. Our results show that the new forecasting system achieves reliable predictions of extreme flood events across different return periods and lead times.

References

[1] Gu, A., and Dao, T.: Mamba: Linear-time sequence modeling with selective state spaces. arXiv preprint arXiv:2312.00752, 2023.

[2] Ho, J., Jain, A., and Abbeel, P.: Denoising diffusion probabilistic models. Advances in neural information processing systems, 33, 6840-6851, 2020.

[3] Nearing, G., Cohen, D., Dube, V. et al. Global prediction of extreme floods in ungauged watersheds. Nature 627, 559–563 2024.

[4] Harrigan, S., Zsoter, E., Cloke, H., Salamon, P., and Prudhomme, C.: Daily ensemble river discharge reforecasts and real-time forecasts from the operational Global Flood Awareness System, Hydrol. Earth Syst. Sci., 27, 1–19, 2023.

How to cite: Shams Eddin, M. H., Zhang, Y., Kollet, S., and Gall, J.: AIFAS: Probabilistic Global River Discharge Forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13844, https://doi.org/10.5194/egusphere-egu25-13844, 2025.

EGU25-14004 | ECS | Posters on site | HS3.4

Learning Basin Similarity Through Combined Deep Learning and Random Forest Approaches for Improved Parameter Transfer in Ungauged Basins 

Rojin Meysami, Qiutong Yu, Bryan Tolson, Hongren Shen, and Rezgar Arabzadeh

Parameter regionalization for ungauged basins remains a critical challenge in hydrological modeling. While traditional approaches rely on physical catchment descriptors or spatial proximity, and recent machine learning applications have focused primarily on direct streamflow prediction, there remains significant potential to leverage machine learning for improved parameter transfer strategies. This study explores novel approaches that combine Long Short-Term Memory (LSTM) networks and Random Forest (RF) models to predict basin similarity and optimize parameter transfer for physically-based hydrologic models. Using case studies from British Columbia's Fraser River Basin and Ontario's Great Lakes region, we test multiple methodologies for integrating deep learning with traditional parameter transfer approaches. Our primary benchmark is established through an exhaustive parameter transfer experiment using the Raven hydrological model, where parameters from each potential donor basin were transferred to every possible receiver basin across 10 independent trials. This benchmark represents the best achievable KGE via parameter transfer methods. Our framework employs a regional LSTM model to capture complex streamflow dynamics and characterize basin similarity, then explores various RF-based approaches to predict optimal donor-receiver basin pairs for parameter transfer. These methods are evaluated against both the exhaustive transfer benchmark and emerging machine learning approaches. Results indicate that thoughtfully combining deep learning and random forest techniques can capture nuanced relationships between basin characteristics and hydrological response similarity, advancing the state-of-the-art in parameter regionalization for ungauged basins while maintaining physical interpretability.

How to cite: Meysami, R., Yu, Q., Tolson, B., Shen, H., and Arabzadeh, R.: Learning Basin Similarity Through Combined Deep Learning and Random Forest Approaches for Improved Parameter Transfer in Ungauged Basins, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14004, https://doi.org/10.5194/egusphere-egu25-14004, 2025.

EGU25-14223 | Orals | HS3.4

On the advancing frontier of deep learning in hydrology:  a hydrologic applications perspective 

Andy Wood, Laura Read, Grey Nearing, Juliane Mai, Chris Frans, Martyn Clark, and Florian Pappenberger

In the last decade, the realization that certain deep learning (DL) architectures are particularly well-suited to the simulation and prediction of hydrologic systems and their characteristic memory-influenced dynamics has led to remarkable rise in DL-centered hydrologic research and applications.  Numerous new datasets, computational and open software resources, and progress in related fields such as numerical weather prediction have also bolstered this growth.  Advances in DL for hydrologic forecasting research and operations is likely the most eye-catching and intuitive use case, but DL methods are now also making inroads into more process-intensive hydrologic modeling contexts, and among groups that have been skeptical of their potential suitability despite performance-related headlines. Nevertheless, even in the forecasting context, and despite offering new strategies and concepts to resolve long-standing hurdles in hydrologic process-based modeling efforts, the uptake of DL-based systems in many public-facing services and applications has been slow. 

This presentation provides perspective on the ways in which DL techniques are garnering interest in traditionally process-oriented modeling arenas -- from flood and drought forecasting to watershed studies to hydroclimate risk modeling – and on sources of hesitancy.  Clear pathways, momentum and motivations for DL approaches to supplant process-based models exist in some applications, whereas in others, governing interests and constraints appear likely to restrict DL innovations to narrower niches.  Concerns over explainability have been a common topic, but less discussed questions about fitness or adequacy for purpose and institutional requirements can also be influential.  Drawing from relevant hydrologic modeling programs, projects and initiatives in the US and elsewhere, we aim to provide a real-world status update on the advancing frontier of deep learning in applied hydrologic science and practice.  

How to cite: Wood, A., Read, L., Nearing, G., Mai, J., Frans, C., Clark, M., and Pappenberger, F.: On the advancing frontier of deep learning in hydrology:  a hydrologic applications perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14223, https://doi.org/10.5194/egusphere-egu25-14223, 2025.

EGU25-15152 | Orals | HS3.4

Evaluation of LSTM Model for Stochastic Discharge Simulation 

Sonja Jankowfsky, Kanneganti Gokul, Shuangcai Li, Arno Hilberts, and Anongnart Assteerawatt

This study evaluates the capacity of a Long Short-Term Memory (LSTM) model trained on a diverse river discharge dataset from over 4,000 USGS gauges across the United States with the aim to generate extremely long stochastic discharge simulations. 

The LSTM model (Kratzert et al., 2022) was trained using 30 years of NLDAS v2 forcings, which were split into 10-year periods for training, validation, and testing respectively. Sixty percent of the gauges had a Nash Sutcliffe Efficiency (NSE) larger than 0.4 in the validation period, and ten percent had an NSE larger than 0.8, which was considered sufficient to proceed with applying the model using stochastic precipitation.  

The stochastic simulations are evaluated in terms of the model’s ability to capture peak discharges. The stochastic return period (RP) curves were evaluated against those from the historical time period and the observed discharge. For most of the gauges, the stochastic RP curves are in line with the historical RP curves, and for all of the gauges, the stochastic RP curves discharge of the extreme return period extend far beyond the discharge of the historical time period, showing the capacity of the model to extrapolate beyond the training dataset. 

This capacity, which is usually lacking in single-basin trained models, most likely results from training on a large dataset with a wide range of climatic conditions and variability as suggested by Kratzert et al. (2024). These findings underscore the robustness and versatility of the LSTM model in long-term stochastic discharge simulations, highlighting its potential for broader hydrological applications. 

Kratzert, F., Gauch, M., Nearing, G., & Klotz, D. (2022). NeuralHydrology — A Python library for Deep Learning research in hydrology. Journal of Open Source Software, 7(71), 4050. https://doi.org/10.21105/joss.04050

Kratzert, F., Gauch, M., Klotz, D., and Nearing, G. (2024). HESS Opinions: Never train an LSTM on a single basin. Hydrology and Earth System Sciences (HESS), Volume 28, Issue 17, published on September 12, 2024.  https://doi.org/10.5194/hess-28-4187-2024.

How to cite: Jankowfsky, S., Gokul, K., Li, S., Hilberts, A., and Assteerawatt, A.: Evaluation of LSTM Model for Stochastic Discharge Simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15152, https://doi.org/10.5194/egusphere-egu25-15152, 2025.

EGU25-15171 | ECS | Posters on site | HS3.4

Learning shallow water equations with physics-informed Deep Operator Network (DeepONet) 

Robert Keppler, Julian Koch, and Rasmus Fensholt

Physics-informed neural networks are an optimization-based approach for solving differential equations and have the potential to significantly speed up the modelling of complex phenomena, which conventionally is achieved via expensive numerical solvers. We present a Physics-Informed Deep Operator Network (DeepONet) framework for solving two-dimensional shallow water equations with variable bed topography under given boundary and initial conditions. While traditional physics-informed neural networks can solve differential equations on meshless grids using prescribed conditions, they require retraining for each new set of initial and boundary conditions. Our approach uses a DeepONet to learn the underlying solution operator rather than individual solutions, which provides an enhanced generalizability, making the DeepONet a feasible candidate for real world applications. The framework combines the advantages of neural networks with physical laws, effectively handling the complexities of varying bed topography and wet-dry transitions. We demonstrate that our DeepONet approach achieves comparable accuracy to classical numerical methods while significantly reducing inference time. In our modelling experiments we investigate the sensitivity of hyperparameter values and network architecture as well as the potential of introducing an additional data loss, emulating the availability of additional observational data on water levels or inundation extent.  This acceleration in computation speed makes the method particularly valuable for time-critical applications such as flood forecasting. The results establish physics-informed DeepONets as a promising alternative to traditional numerical solvers for shallow water systems, offering a balance between computational efficiency and solution accuracy.

How to cite: Keppler, R., Koch, J., and Fensholt, R.: Learning shallow water equations with physics-informed Deep Operator Network (DeepONet), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15171, https://doi.org/10.5194/egusphere-egu25-15171, 2025.

EGU25-15229 | ECS | Posters on site | HS3.4

Cryosphere Data and Its Value for Deep Learning Hydrological Simulations 

Corinna Frank, Jan Philipp Bohl, Manuela Brunner, Martin Gauch, and Marvin Höge

Deep learning models have been successfully applied to simulate streamflow in mountain catchments. While these mostly lumped models have demonstrated the ability to learn processes such as snow accumulation and melt that are crucial for streamflow generation in these regions, they still show deficiencies in simulating streamflow during the melting period. This suggests a misrepresentation of melting dynamics encoded within these models. We hypothesize that the sets of lumped meteorological variables (such as air temperature, precipitation, PET) and static attributes currently used to train and drive these models are not sufficient to describe the melting processes. 

To enhance the representation of snow and ice-related processes, we thus propose to incorporate additional data on snow and ice cover, such as Snow Covered Area, Snow Water Equivalent, and glacier mass within the respective basin. We assess (1) how much additional value can be extracted from cryosphere data to improve the representation of cryosphere related processes and (2) how the added value varies across different geographies and catchment types. In a lumped Long Short-Term Memory (LSTM) setup covering a large sample of catchments in different European mountainous regions, we compare different data integration methods with respect to their uncertainty reduction for streamflow simulation and their limitations for model applications.
Our findings provide insights into optimizing model configurations and data usage and offer practical guidance for ultimately improving the accuracy of streamflow simulations in mountainous, snow-influenced regions. 

How to cite: Frank, C., Bohl, J. P., Brunner, M., Gauch, M., and Höge, M.: Cryosphere Data and Its Value for Deep Learning Hydrological Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15229, https://doi.org/10.5194/egusphere-egu25-15229, 2025.

EGU25-15350 | ECS | Posters on site | HS3.4

Graph-Based Representations in Hydrological Modeling: Comparing SWAT+ and Graph Neural Networks for Water Management Systems 

Moritz Wirthensohn, Ye Tuo, and Markus Disse

Extreme hydrological events such as droughts and floods are expected to become more frequent and severe according to climate change projections, making effective water management very important to mitigate environmental and socio-economic impacts. In this context, advanced hydrological modeling tools are essential for understanding and managing water systems. The Soil and Water Assessment Tool (SWAT+), a process-based and semi-distributed eco-hydrological model, has become very popular for simulating hydrological processes and water management scenarios, especially with its improved water allocation and reservoir modules. At the same time, Graph Neural Networks (GNNs), a deep learning model, have shown potential for modeling complex relationships in networked systems. Both SWAT+'s water allocation module and GNNs use graph-like structures to model water systems. The goal of this study is to systematically compare the structural components of these two approaches and provide insights into potential integration.

Using the Upper Isar River Basin's complex water management system as a case study, we examine how SWAT+ and GNNs can be used to model it. We perform a component-wise analysis, focusing on how these models can represent nodes, edges, and attributes in a networked water management system. While this study focuses on structural rather than performance comparisons, we anticipate that our results will highlight the strengths and limitations of each approach. SWAT+ is expected to excel at incorporating domain-specific knowledge and explicitly representing management actions. GNNs could provide advantages in learning complex patterns from data and faster simulations for larger catchments.

The findings could open the way for hybrid approaches that combine traditional hydrological models' strengths with GNNs' learning capabilities. This could lead to more robust and adaptable water management tools to deal with the growing complexity of hydrological systems caused by climate change and human intervention.

How to cite: Wirthensohn, M., Tuo, Y., and Disse, M.: Graph-Based Representations in Hydrological Modeling: Comparing SWAT+ and Graph Neural Networks for Water Management Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15350, https://doi.org/10.5194/egusphere-egu25-15350, 2025.

Accurate reservoir outflow simulation is crucial for modeling streamflow in reservoir-regulated basins. In this study, we introduce a knowledge-guided Long Short-Term Memory model (KG-LSTM) to simulate the outflow of reservoirs-Fengshuba, Xinfengjiang, and Baipenzhu in the Dongjiang River Basin, China. KG-LSTM is built on the standard hyperparameters-optimized-LSTM and the loss function considering reservoir operation knowledge, while traditional reservoir model level pool scheme (LPS) is used as a benchmark model. Model uncertainty is analyzed using the bootstrap method. We then propose a hybrid approach that combines KG-LSTM with the Three-parameter monthly hydrological Model based on the Proportionality Hypothesis (KG-LSTM-TMPH) for streamflow simulation. The propagation of inflow errors to outflow simulations is studied across the three reservoirs. Results indicate that LSTM-based models greatly outperform LPS in all three reservoirs, with KG-LSTM demonstrating superior capability in capture reservoir outflow dynamics compared to the standard LSTM model. In the multi-year regulated Xinfengjiang Reservoir, KG-LSTM improves Nash-Sutcliffe efficiency (NSE) from 0.59 to 0.64, and reduces root mean squared error (RMSE) from 55.59 m³/s to 54.84 m³/s during the testing period. KG-LSTM shows reduced model uncertainty, decreasing the relative width (RW) from 0.55 to 0.51 in the Xinfengjiang Reservoir and from 0.48 to 0.44 in the Baipenzhu Reservoir, while demonstrating limited change in the Fengshuba Reservoir. For streamflow simulation, KG-LSTM-TMPH performs best across all four stations, achieving NSE values of approximately 0.87, 0.88, 0.91, and 0.92 at Longchuan, Heyuan, Lingxia, and Boluo stations, respectively. In the dry season, KG-LSTM-TMPH demonstrates substantial improvement over LSTM-TMPH, increasing R² by +0.11 and reducing RMSE by -4.22 m³/s at Heyuan station. Inflow errors impact outflow most significantly for the Xinfengjiang Reservoir in April and May, for the Fengshuba Reservoir throughout the year (particularly in April, May, July, and August), and for the Baipenzhu Reservoir primarily in July and August. This study enhances reservoir outflow modeling by integrating reservoir operation knowledge with deep learning. The hybrid KG-LSTM-TMPH approach shows practical potential for streamflow simulation in reservoir-regulated basins, offering valuable applications for water resource management.

How to cite: Wang, D.: A Knowledge-guided LSTM reservoir outflow model and its application to streamflow simulation in reservoir-regulated basins, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16156, https://doi.org/10.5194/egusphere-egu25-16156, 2025.

EGU25-16414 | Posters on site | HS3.4

Exploring the Limits of Spatial Generalization Ability in Deep Learning Models for Hydrology 

Benedikt Heudorfer, Hoshin Gupta, and Ralf Loritz

State-of-the-art deep learning models for streamflow prediction (so-called Entity-Aware models, EA) integrate information about physical catchment properties (static features) with climate forcing data (dynamic features) from multiple catchments simultaneously. However, recent studies challenge the notion that this approach truly leverages generalization ability. We explore this issue by conducting experiments running Long-Short Term Memory (LSTM) networks across multiple temporal and spatial in-sample and out-of-sample setups using the CAMELS-US dataset. We compare LSTMs equipped with static features with ablated variants lacking these features. Our findings reveal that the superior performance of EA models is primarily driven by meteorological data, with negligible contributions by static features, particularly in spatial out-of-sample tests. We conclude that EA models cannot generalize to new locations based on provided physical catchment properties. This suggests that current methods of encoding static feature information in our models may need improvement, and that the quality of static features in the hydrologic domain might be limited. We contextualize our results with observations made in the broader deep learning field, which increasingly grapples with the challenges of (lacking) generalization ability in state-of-the-art deep learning models.

How to cite: Heudorfer, B., Gupta, H., and Loritz, R.: Exploring the Limits of Spatial Generalization Ability in Deep Learning Models for Hydrology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16414, https://doi.org/10.5194/egusphere-egu25-16414, 2025.

EGU25-19190 | ECS | Orals | HS3.4

Application of Attention-Based Graph Neural Networks for Spatial Distribution Prediction of Streamflow 

Xian Wang, Xuanze Zhang, and Yongqiang Zhang

Accurate streamflow estimation is crucial for effective water resource management and flood forecasting. However, physics-based hydrological models fail to respond promptly to rapid hydrological events due to lack efficiency in model calibration and computing time for large-scale catchment , while existing deep learning models tend to neglect the physical processes of runoff transfer, failing to account for the spatial and temporal dependencies inherent in runoff dynamics. In this study, we propose a topological process-based model that integrates Graph Attention Networks (GAT) to capture the spatial topology of runoff transfer and Long Short-Term Memory (LSTM) networks to simulate the temporal transfer between upstream and downstream runoff. The model was applied to the Yangtze River Basin which is the largest river basin in China to predict streamflow at 10 km spatial resolution. Validation results show that our model achieves a median Nash-Sutcliffe Efficiency (NSE) value of 0.783 at secondary outlet stations across the basin and effectively simulates the streamflow peak due to flooding. Additionally, the model is capable of simulating the spatial distribution of daily streamflow for an entire year within 10 seconds, providing a significant computational speedup compared to physical process-based river confluence models. This work represents a step towards more efficient and responsive prediction of extreme hydrological events using deep learning model.

How to cite: Wang, X., Zhang, X., and Zhang, Y.: Application of Attention-Based Graph Neural Networks for Spatial Distribution Prediction of Streamflow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19190, https://doi.org/10.5194/egusphere-egu25-19190, 2025.

EGU25-19716 | ECS | Orals | HS3.4

Leveraging Machine Learning to Uncover and Interpret Relevant Catchment Features  

Alberto Bassi and Carlo Albert

Recent advances in catchment hydrology [Kratzert et al., 2019–2021] demonstrate the superiority of LSTMs over traditional conceptual models for streamflow prediction in large-sample datasets. LSTMs achieve better streamflow accuracies by leveraging information from diverse hydrological behaviors. These models are enriched with static catchment attributes, which, when combined with meteorological drivers, play a critical role in streamflow formation. Augmenting LSTMs with these attributes further enhances their performance compared to vanilla LSTMs, underscoring the importance of these attributes for accurate streamflow predictions. Building on this, a recent study [Bassi et al., 2024] employed a conditional autoencoder to reveal that most of the relevant catchment information for streamflow prediction can be distilled into two features, with a third feature being beneficial for particularly challenging catchments. In this work, we directly derive a minimal set of catchment features from known attributes by passing them through the encoder and subsequently comparing streamflow predictions against state-of-the-art benchmarks [Kratzert et al., 2021]. Our findings indicate that while the intrinsic dimension of 26 commonly used attributes is four, only two features suffice for accurate streamflow prediction. This aligns closely with the findings of Bassi et al. (2024), suggesting that nearly all relevant information for streamflow prediction is encapsulated in known attributes. Finally, we provide an interpretation of these two machine-learning-derived features using information theory techniques.

How to cite: Bassi, A. and Albert, C.: Leveraging Machine Learning to Uncover and Interpret Relevant Catchment Features , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19716, https://doi.org/10.5194/egusphere-egu25-19716, 2025.

Continuum sea-ice models are increasingly being applied to high-resolution settings, while there are still open questions about the physics governing sea-ice deformation on these resolutions. Simultaneously, discrete element method (DEM) models are now starting to be used to address questions regarding specific processes within sea-ice deformation. A direct comparison of both methods has not been done yet, as the spatial resolution differs on several orders of magnitude and the computational costs of high-resolution DEM simulations over large areas of sea ice are high. Here, we will present a comparison of idealized simulations of sea-ice convergence utilizing both methods. We used the neXtSIM sea-ice model as the continuum model and HiDEM as the DEM model. Sea-ice deformation in neXtSIM is determined by a brittle rheology with Lagrangian sea-ice advection. In HiDEM, the ice is described by spherical particles connected by beams, which can fail as the ice cover locally reaches a critical stress state. In both cases, we simulate the same sea-ice area and use the same forcing, yet the spatial resolution differs. This setup enables us to investigate the sea-ice deformation yielding from both methods. We compare the resulting ice thickness distributions and ice ridge formation patterns and highlight the similarities and differences between both methods.

How to cite: Muchow, M., Ólason, E., and Polojärvi, A.: Exploratory sea-ice simulations: Comparing idealized sea-ice compression simulations using a continuum and discrete element method models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-130, https://doi.org/10.5194/egusphere-egu25-130, 2025.

EGU25-1585 | ECS | Posters on site | CR3.2

A New Parameterization of Dilation Using GODAR 

Antoine Savard, Bruno Tremblay, and Arttu Polojärvi

Capturing all sea ice dynamical aspects in a model is notoriously challenging due to the complex interplay of granular and fracture-dominated processes. In the central Arctic, linear kinematic features (LKFs) dominate deformation patterns, while the marginal ice zone (MIZ) is characterized by fragmented floes where the collisional mode is dominant. The rheological properties of sea ice in these region differ significantly, and a rheological model that could be used in all regimes is desirable. Continuum models, commonly used for large-scale sea ice simulations, rely on parameterizations to approximate subgrid-scale processes such as floe interactions, wave attenuation, and dilation. Although high-resolution (<2 km) continuum models improve the representation of LKFs and deformation statistics, they remain fundamentally limited by their reliance on simplified, or ill-posed rheologies and the continuum assumption, which cannot reconcile velocity discontinuities inherent in granular materials like sea ice. Discrete element models (DEMs), on the other hand, explicitly resolve particle-scale interactions and naturally capture fracture and granular behaviour, but their computational cost has historically restricted their application to small-scale scenarios.

We addressed this gap by developing the granular floes for discrete Arctic rheology (GODAR) model, a DEM specifically designed to simulate the mesoscale evolution of sea ice mechanics. GODAR tracks the time evolution of contact normals between floes, enabling us to derive generalized equations that relate dilation to prognostic variables such as shear and normal stress, open water fraction, and floe size distribution. These results demonstrate that GODAR effectively captures both the granular physics and fracture-driven dynamics underpinning LKFs. By seamlessly integrating microscale processes into macroscale behaviour, GODAR offers a powerful framework for bridging the limitations of continuum models. Its insights provide a pathway to improved parameterizations, advancing both the scientific understanding of sea ice dynamics and the operational forecasting capabilities necessary for safe navigation and climate modeling.

How to cite: Savard, A., Tremblay, B., and Polojärvi, A.: A New Parameterization of Dilation Using GODAR, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1585, https://doi.org/10.5194/egusphere-egu25-1585, 2025.

Reliable prediction of short-term Arctic sea ice variation is crucial for ensuring the safety of navigation on Arctic shipping routes. While deep-learning models have demonstrated potential in improving the accuracy of sea ice predictions, many data-driven approaches focus solely on individual aspects of sea ice without considering the interrelationships and underlying physical laws governing various sea ice factors. To address this limitation, we introduce a dual-task prediction model that simultaneously targets sea ice concentration (SIC) and sea ice motion (SIM). Our approach incorporates a novel loss function that enforces dynamic constraints derived from the sea ice control equation, ensuring that predictions of both SIC and SIM are consistent with physical dynamics. We conduct comprehensive comparative experiments to identify the optimal model structure for predicting SIC and SIM. Our findings reveal that a dual-task branching architecture is particularly effective for this purpose, with a post-decoder branch network structure exhibiting the best performance in predicting both SIC and SIM. By integrating the sea ice dynamics equation into the loss function, our models demonstrate enhanced alignment with physical laws, leading to improved predictability and accuracy in SIC and SIM prediction.

How to cite: Wang, Y. and Liu, Q.: Physics-Embedded Deep Convolutional Network: A Novel Approach for Prediction of Sea Ice Concentration and Motion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3643, https://doi.org/10.5194/egusphere-egu25-3643, 2025.

EGU25-4127 | ECS | Orals | CR3.2

Data-driven equation discovery of a sea ice albedo parametrisation 

Diajeng Atmojo, Katja Weigel, Arthur Grundner, Marika Holland, and Veronika Eyring

In the sea ice model Finite-Element Sea Ice Model (FESIM), a part of the Finite-Element Sea ice Ocean Model (FESOM), sea ice albedo is treated as a tuning parameter defined by four constant values depending on snow cover and surface temperature. This parametrisation is too simple to capture the spatiotemporal variability in sea ice albedo observed via satellites. Our work aims to improve this parametrisation by discovering an interpretable, physically-consistent equation for sea ice albedo using symbolic regression, an interpretable machine learning technique, combined with physical constraints. Leveraging pan-Arctic satellite and reanalyses data from 2013 to 2020, we apply sequential feature selection to identify the most informative input variables for sea ice albedo. With sequential feature selection, we develop parsimonious models that perform well with as few input variables as possible. To understand how additional model complexity reduces error, we evaluate our discovered equations against baseline models with different complexities, such as multilayer perceptron neural networks and polynomials on an error-complexity plane, identifying the models on the Pareto front. Our results indicate that parsimonious models demonstrate better generalisation to unseen data than models using the full set of input variables. Compared to the current FESIM parametrisation, our best equation reduces the mean squared error by about 51%, while excelling in balancing error and complexity. Unlike neural networks, our equation allows for further regional and seasonal analyses due to its inherent interpretability by fine-tuning the coefficients representing the weights of each term and input variable. Through the synergy of observations with machine learning, we aim to deepen the process-level understanding of the Arctic Ocean’s surface radiative budget and reduce uncertainty in climate projections.

How to cite: Atmojo, D., Weigel, K., Grundner, A., Holland, M., and Eyring, V.: Data-driven equation discovery of a sea ice albedo parametrisation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4127, https://doi.org/10.5194/egusphere-egu25-4127, 2025.

EGU25-4696 | Posters on site | CR3.2

High-resolution large-scale model for sea ice dynamics 

Arttu Polojärvi, Jan Åström, and Jari Haapala

Forecasts of sea-ice motion and deformation are crucial for maritime operations including winter navigation and offshore wind energy harvesting. Further, sea-ice models have a key role in predictions on long-term effects of climate change. In this study we utilize the Helsinki Discrete Element Model (HiDEM) to simulate sea-ice breakup and dynamics. HiDEM code is optimized for high-performance supercomputers and achieves superior temporal and spatial resolutions when compared to conventionally used continuum models. We compare simulated fracture patterns and ice motion with satellite images from the Kvarken region of the Baltic Sea and show that HiDEM reproduces observed ice deformation patterns, which formed over a period of few days in nature. The results closely match the observed ice fracture and motion patterns, floe sizes, ridge structures, and fast-ice regions. The simulations cover an area of about 100 km × 100 km with 8 m resolution and they completed in about 10 hours of wall clock time.

How to cite: Polojärvi, A., Åström, J., and Haapala, J.: High-resolution large-scale model for sea ice dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4696, https://doi.org/10.5194/egusphere-egu25-4696, 2025.

EGU25-7735 | Orals | CR3.2

Ultra-high resolution pan-Arctic sea ice-ocean coupled simulation on a heterogeneous many-core supercomputer 

Longjiang Mu, Yuhu Chen, Hong Wang, Ruizhe Song, Lin Zheng, and Xianyao Chen

Arctic sea ice has undergone dramatic changes in recent decades. The decline in sea ice thickness has resulted in more brittle ice, which is increasingly susceptible to deformation by wind and ocean currents. Small-scale features such as sea ice leads and ridges are frequently observed in the field but remain poorly understood. Accurately forecasting these features requires high-resolution sea ice modeling with a horizontal resolution of several kilometers. To address this, a pan-Arctic ultra-high-resolution (~500 m) sea ice-ocean coupled model has been developed. This model is based on the Massachusetts Institute of Technology General Circulation Model (MITgcm) but has been substantially refactored and enhanced to adapt to the heterogeneous many-core architecture of the computing system. The model's Pacific open boundary is positioned north of the Okhotsk Sea, away from the Aleutian Islands, while the Atlantic open boundary is set north of the Strait of Gibraltar to avoid the influence of deep convection processes. The model operates on a three-dimensional grid comprising approximately 15.1 billion points, with around 9 billion wet points. The sea ice component shares the same grid as the ocean model, enabling direct coupling between the two at each grid point. For sea ice thermodynamics, a zero-heat-capacity, one-layer model is employed, while sea ice dynamics are governed by viscous-plastic rheology. The highly nonlinear sea ice momentum equations are solved using a tridiagonal solver combined with a line successive relaxation method, achieving an accuracy of 1.0×10⁻⁵. The nonlinear integration is iterated 10 times, with each iteration allowing a maximum of 500 steps to ensure convergence of the high-resolution solutions. The model demonstrates significant improvements in simulating sea ice ridges compared to lower-resolution models. Validation against IceSAT-2 along-track data reveals strong agreement in both spatial distribution and probability density function, underscoring the model's enhanced capability to capture small-scale sea ice features.

How to cite: Mu, L., Chen, Y., Wang, H., Song, R., Zheng, L., and Chen, X.: Ultra-high resolution pan-Arctic sea ice-ocean coupled simulation on a heterogeneous many-core supercomputer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7735, https://doi.org/10.5194/egusphere-egu25-7735, 2025.

EGU25-8384 | ECS | Posters on site | CR3.2

Who causes whom? A spatially distributed causal analysis of the relationship between Arctic sea ice and teleconnection indices 

Guido Ascenso, Matteo Sangiorgio, Ian Baxter, and Andrea Castelletti

The relationship between Arctic sea ice and tropical climate variability is a crucial aspect of global climate dynamics. While numerous studies have explored potential links between sea ice concentration (SIC) or sea ice thickness (SIT) and teleconnection indices such as AMO, AO, NAO, ENSO, and PDO, these investigations often faced challenges in fully capturing the complexity of these interactions. For instance, most analyses relied on linear, non-causal methods such as trend matching (although the underlying processes are likely highly nonlinear), or focused on single indices (thus potentially missing more complex interactions when more than one index is considered at once), or analyzed the relationship in aggregate over the entire Arctic region, rather than considering subtle regional differences. Additionally, these teleconnections were often assessed in only one “direction” (e.g., how much ENSO influences SIC), but there is evidence to suggest that there may be two-way interactions at play.

In this study, we address these challenges by proposing a bi-directional, causal, and spatially distributed approach to analyze the relationships between SIC/SIT and eight teleconnection indices. Using transfer entropy (TE), a non-parametric measure of information flow, we quantify the influence of these indices on SIC/SIT and vice versa across multiple lead times. This approach lets us understand how these causal relationships vary at different lead times and over different Arctic regions, to verify whether the various teleconnection indices provide information that is complementary or redundant, and to detect preferential directions in the causal relationship between indices and ice (thus answering the question “who influences whom?”). For instance, our results indicate that the North Atlantic Oscillation is influenced by the Arctic ice more than it itself affects the ice, whereas the relationship is inverted for the Atlantic Multidecadal Oscillation.

Although we focus our analysis on understanding the spatial and temporal variability of Arctic-teleconnection interactions, the proposed framework is highly flexible and can be adapted to consider other indices and lead times, and entirely different domains altogether.

How to cite: Ascenso, G., Sangiorgio, M., Baxter, I., and Castelletti, A.: Who causes whom? A spatially distributed causal analysis of the relationship between Arctic sea ice and teleconnection indices, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8384, https://doi.org/10.5194/egusphere-egu25-8384, 2025.

EGU25-9952 | ECS | Orals | CR3.2

Linking the evolution of floe-scale ice characteristics to its deformation history using satellite observations 

Nils Hutter, Cecilia Bitz, and Luisa von Albedyl

Arctic sea ice is a mosaic of ice floes whose distribution and thicknesses greatly impact the interaction of sea ice with the atmosphere and the ocean. However, we are still lacking knowledge of the physics to describe the complex interplay of ice floes that are a key characteristic of sea ice. In our contribution, we outline a framework to characterize sea-ice deformation at the floe-scale from observational data by studying the mechanical interaction of multiple identifiable floes. We use Sentinel SAR imagery and ICESat-2 data acquired during the MOSAiC expedition to map ice floes and their thickness in the larger area around Polarstern. This combination of data products allows us to describe the floe-size distribution of floe diameters from tens of kilometers down to tens of meters. With the repeated coverage of SAR imagery, ice motion is tracked and deformation estimates are derived. By combining both floe-size estimates and deformation rates we provide insights into how the floe composition changes in regions that were exposed to deformation and highlight ice fracture as a major source of the power-law distribution of floe sizes. Finally, we present a parameterization of this relationship between floe sizes and ice fracture for large-scale continuum sea-ice models.

How to cite: Hutter, N., Bitz, C., and von Albedyl, L.: Linking the evolution of floe-scale ice characteristics to its deformation history using satellite observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9952, https://doi.org/10.5194/egusphere-egu25-9952, 2025.

EGU25-11839 | ECS | Posters on site | CR3.2

Modeling Fast Ice in the Southern Ocean Using a Particle-Continuum Approach 

Carolin Mehlmann

Approximately 4% to 13% of sea ice remains stationary, forming a narrow band around Antarctica. This contrasts with the majority of sea ice, which drifts with winds and ocean currents as "pack ice." This stationary landfast sea ice, known as "fast ice," is anchored to the coastline or grounded by icebergs and has significant implications for the global climate. However, current global climate models poorly represent fast ice, casting doubt on their ability to make accurate future projections for this critical component.

To address this limitation, we have developed a prognostic fast-ice representation suitable for coupled climate models. Our approach introduces a novel coupling mechanism between sea ice and grounded icebergs. This mechanism incorporates feedback from subgrid-scale grounded iceberg particles into the sea ice rheology. Idealized test cases demonstrate that this method successfully simulates fast ice as well as coastal polynyas due to subgrid-scale iceberg grounding.

How to cite: Mehlmann, C.: Modeling Fast Ice in the Southern Ocean Using a Particle-Continuum Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11839, https://doi.org/10.5194/egusphere-egu25-11839, 2025.

EGU25-12073 | ECS | Posters on site | CR3.2

Arctic landfast ice simulation with brittle rheology and probabilistic grounding 

Augustin Lambotte, Thierry Fichefet, François Massonnet, Laurent Brodeau, Pierre Rampal, Jean-François Lemieux, and Frédéric Dupont

Landfast ice, i.e., sea ice that is mechanically immobilized for several weeks along the coasts, significantly influences the underlying ocean by controlling the occurrence of coastal polynyas and the formation of dense water within. However, it is usually poorly represented in numerical models. In the Arctic, the accurate simulation of landfast ice relies on parameterizing sea ice grounding in shallow water areas and on the sea ice rheology capability to form ice arches in regions with restricted geometry. In this study, we compare a brittle rheology (i.e., the Brittle Bingham-Maxwell or BBM one), newly implemented in the ocean-sea ice model NEMO-SI3, with a standard viscous-plastic rheology (i.e., the aEVP), which is widely used in sea ice models. The performance of the two rheologies in forming ice arches and landfast ice is evaluated at the scale of the Arctic at a 0.25° horizontal resolution. For the grounding parameterization, we apply a probabilistic grounding scheme based on the ice thickness distribution and investigate how leveraging subgrid-scale bathymetry statistics can enhance its performance.

How to cite: Lambotte, A., Fichefet, T., Massonnet, F., Brodeau, L., Rampal, P., Lemieux, J.-F., and Dupont, F.: Arctic landfast ice simulation with brittle rheology and probabilistic grounding, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12073, https://doi.org/10.5194/egusphere-egu25-12073, 2025.

EGU25-12255 | Orals | CR3.2

A unified sea ice fracture model for climate applications 

Bruno Tremblay and Lettie Roach

Interactions between ocean surface waves and sea ice dictate the width of the marginal ice zone, where new ice formation and increased sea ice melt are present in the winter and summer (respectively). Existing sea ice wave fracture models predict fracture when one of two limits is reached: (i) a maximum strain failure criterion assuming that the ice is a perfectly flexible plate that follows the ocean surface, and (ii) a maximum stress failure criterion assuming that the ice is a perfectly rigid plate that does not deform under the action of buoyancy and gravity forces. The perfectly rigid sea ice plate model is valid for small wavelengths that have a short lever arm but systematically predicts fracture for long wavelengths irrespective of the amplitude because of the long lever arm. Conversely, the flexible plate model is valid for long wavelengths but systematically predicts fracture for short wavelengths because of the unrealistically large strain. In this work, we present a unified sea ice fracture model based on elastic beam theory for the bending of a sea ice plate (or floe) that is valid for all wavelengths. Our approach reduces to the rigid plate and fully flexible model for short and long incoming ocean wavelength limits, respectively. Results using a fully-developed ocean wave field show much smaller strain within the ice plate and a resulting floe size distribution after fracture with a higher mean and no floes in the smallest size categories. This distribution also aligns with correct ice thickness and Young's Modulus dependencies, matching observational evidence, and contrasts with results from perfectly rigid or flexible sea ice plate models.

How to cite: Tremblay, B. and Roach, L.: A unified sea ice fracture model for climate applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12255, https://doi.org/10.5194/egusphere-egu25-12255, 2025.

EGU25-12835 | ECS | Orals | CR3.2

Fast, flexible, focused: the case for a single-column sea ice data assimilation framework 

Molly Wieringa, Joseph Rotondo, Christopher Riedel, Jeffrey Anderson, and Cecilia Bitz

Assimilating sea ice observations into numerical sea ice and climate models has garnered increasing interest, driven by a demand for more comprehensive sea ice records and forecasts in response to a rapidly changing cryosphere. The development of data assimilation (DA) techniques targeted specifically for sea ice, however, has been comparatively limited.  The computational requirements and structure of many modern sea ice models, the physical characteristics of key sea ice variables, and the uncertainty and relatively limited scope of assimilated sea ice observations all pose significant challenges for the development and tuning of sea ice DA systems. This work presents a new, lightweight framework for sea ice DA development that couples a flexible ensemble DA software to a single-column, multi-category sea ice model, and reviews several recent applications. Key results include the variable impact of common sea ice observation kinds across different sea ice regime types; the benefits of tailoring DA algorithms to the physical and modeled characteristics of sea ice; and the efficacy of assimilating new kinds of observations, including the ice thickness distribution and sea ice albedo. Collectively, these results highlight the ease of experimentation proffered by this new framework, which enables both novel research and more accessible development in sea ice state estimation and forecasting contexts.

How to cite: Wieringa, M., Rotondo, J., Riedel, C., Anderson, J., and Bitz, C.: Fast, flexible, focused: the case for a single-column sea ice data assimilation framework, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12835, https://doi.org/10.5194/egusphere-egu25-12835, 2025.

EGU25-13483 | ECS | Orals | CR3.2

A multi-scale approach to model ice mélange 

Saskia Kahl and Carolin Mehlmann

The continuum viscous-plastic sea-ice model is widely used in climate models for simulating large-scale sea-ice dynamics, usually on grids of several kilometres (> 10km). Recently, there is an increasing interest in modelling small-scale processes that have the potential to impact large-scale dynamics, such as sea-ice iceberg interactions in the context of ice mélange. Ice mélange has not yet been studied in the context of climate models as efficient numerical realizations are missing. To close this gap, we present a hybrid ice-mélange model. In this approach, icebergs in form of particles are coupled to the viscous-plastic sea-ice model by modifying the tensile strength in the presence of icebergs. The icebergs, in the size of several hundreds of meters, are tracked on a subgrid scale, which makes the approach numerically efficient. Based on a series of idealised test cases, we demonstrate that this approach captures relevant small-scale physics such as polynya formation caused by grounded icebergs. 

How to cite: Kahl, S. and Mehlmann, C.: A multi-scale approach to model ice mélange, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13483, https://doi.org/10.5194/egusphere-egu25-13483, 2025.

EGU25-14272 | Posters on site | CR3.2

Observational Requirements in the Context of AI prediction Systems - a PCAPS ORCAS Task Team 

Clare Eayrs and Lorenzo Zampieri

The PCAPS ORCAS task team is part of the WMO's World Weather Research Programme's PCAPS (Polar Coupled Analysis and Prediction for Services) project. PCAPS builds upon the foundational work of the Polar Prediction Project and its flagship activity, the Year of Polar Prediction, to improve the actionability, impact, and fidelity of environmental forecasting for human and environmental well-being in the Arctic and Antarctic regions. PCAPS ORCAS is a community effort that aims to enhance forecasting capabilities by exploring the potential of new AI techniques. Outcomes from this initiative will contribute to strengthening observing systems, including satellite and field campaign data, to provide better initialisation and validation for sea-ice forecasts. 

Recent advances in artificial intelligence are transforming sea-ice forecasting, with AI models demonstrating comparable or superior performance to traditional physics-based approaches while requiring significantly fewer computing resources. These advantages could enable more frequent and timely predictions, benefiting stakeholders. However, the effective development and validation of these AI systems depend heavily on high-quality observational data. AI models are generally trained on reanalysis datasets, and data from observational campaigns--though vital for process understanding--has seen limited integration into these products. Such observations are essential to evaluate the physical realism of AI models and build trust in their predictive capabilities.

The PCAPS ORCAS task team systematically evaluates the observational requirements necessary for next-generation AI-based sea-ice prediction systems. This effort combines historical campaign data analysis with collaborative AI model assessments, focusing particularly on extreme events captured during major observational campaigns such as MOSAiC. We examine how different types of observational data contribute to model initialisation and validation while assessing the physical consistency of AI predictions compared to traditional forecasting systems. 

This approach identifies critical gaps in current observing systems and will inform the design of future field campaigns and observation networks, including those proposed for Antarctica InSync and the upcoming fifth International Polar Year. Our recommendations for strengthening polar observing systems specifically address the unique requirements of AI-based prediction systems while maintaining physical consistency in forecasts. These insights are essential for the polar science community as we work to improve the accuracy and reliability of sea-ice predictions in a rapidly changing Arctic and Antarctic environment.

How to cite: Eayrs, C. and Zampieri, L.: Observational Requirements in the Context of AI prediction Systems - a PCAPS ORCAS Task Team, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14272, https://doi.org/10.5194/egusphere-egu25-14272, 2025.

EGU25-16681 | ECS | Orals | CR3.2

Multivariate surrogate model of sea ice in the Arctic region  

Flavia Porro, Charlotte Durand, Tobias Sebastian Finn, Marc Bocquet, Alberto Carrassi, and Pierre Rampal

The rapid changes occurring in Arctic sea ice influence climate and marine ecosystems, mid-latitude weather on timescales from weeks to months, and human activities, further motivating the need for accurate forecasts. A novel generation of sea ice models based on Elasto-Brittle rheologies, such as neXtSIM (Rampal et al, 2016), successfully represents sea-ice processes, with a remarkable accuracy at the mesoscale, for resolutions of about 10 km. However, these models are computationally expensive, limiting their practical application for long-term forecasting. To address this challenge, we leverage deep learning techniques to build an accurate and computationally affordable surrogate of the physical model.  

Following up from the initial work by Durand et al., 2024 on univariate surrogate of the sea-ice thickness (SIT) in neXtSIM, we present here a multivariate surrogate model designed to emulate simultaneously SIT, sea-ice concentration (SIC), and sea-ice velocities (SIU and SIV) in the Arctic region. As its core, our deterministic neural-network-based surrogate model uses a U-Net architecture, tailored to the sea-ice forecasting problem. The model is trained on reforecast-like data generated from neXtSIM and atmospheric forcings from ERA5, which help the model to better represent advective and thermodynamic processes. The neural network is trained to predict sea-ice fields with a 12-hour lead time, and it can iteratively be applied to extend predictions for up to a year. 

We thoroughly investigate the learning process, providing a detailed analysis of our choice of customized loss function and its optimal parameter values. In particular, we investigate the importance of each predicted variable and perform a feature sensitivity analysis. The forecast skills of our model have been successfully evaluated for lead times of up to one year, using both statistical and physical-dynamical metrics. Our preliminary results indicate that the model demonstrates good prediction capabilities at much lower computational costs than the original physical model. The application of a supervised deep learning approach to sea-ice modeling offers a promising alternative to traditional, computationally intensive methods. The positive results from our model's predictions underscore its potential as a reliable tool for seasonal sea ice forecasting. 

 

Rampal P. et al. “neXtSIM: a new Lagrangian sea ice model”. In: The Cryosphere 10.3 (2016), pp. 1055–1073 

Durand C. et al. “Data-driven surrogate modeling of high-resolution sea-ice thickness in the Arctic”. In: The Cryosphere 18.4 (2024), pp 1791-1815 

How to cite: Porro, F., Durand, C., Finn, T. S., Bocquet, M., Carrassi, A., and Rampal, P.: Multivariate surrogate model of sea ice in the Arctic region , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16681, https://doi.org/10.5194/egusphere-egu25-16681, 2025.

EGU25-20343 | ECS | Orals | CR3.2

An analog experiment of sea-ice fracture by waves at the laboratory scale. 

Baptiste Auvity, Laurent Duchemin, Antonin Eddi, and Stéphane Perrard

We study at the laboratory scale the rupture of thin floating sheets made of a brittle material under wave induced mechanical forcing. We show that the rupture occurs where the curvature is maximum, and the break up threshold strongly depends on the wave properties. We observe that the corresponding critical stress for fracture depends on the forcing wavelength: our observations are thus incompatible with a critical stress criteria for fracture. Our measurements can rather be rationalized using an energy criteria: a fracture propagates when the material surface energy is lower than the released elastic energy, which depends on the forcing geometry. I will eventually discuss the possible implication for sea ice fracture criterion by ocean waves.

How to cite: Auvity, B., Duchemin, L., Eddi, A., and Perrard, S.: An analog experiment of sea-ice fracture by waves at the laboratory scale., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20343, https://doi.org/10.5194/egusphere-egu25-20343, 2025.

EGU25-21072 | Orals | CR3.2

Influence of Snow Redistribution and Melt Pond Schemes on Sea Ice Thickness Simulation during MOSAiC Expedition 

Yang Lu, Jiawei Zhao, Xiaochum Wang, and Ralf Giering

The Multidisciplinary drifting Observatory for the Study of Arctic Climate (MOSAiC) expedition was implemented with one year observation of atmosphere, ocean and sea ice, giving us an opportunity to understand the sea ice processes. Due to the missing observation during the expedition, ERA5 atmospheric reanalysis along the MOSAiC drift trajectory, after its validation, is used to force a column sea ice model Icepack, commonly used in coupled climate models. We compare sea ice thickness (SIT) simulations against MOSAiC observation to understand the reasons of SIT simulation misfits fordifferent combinations of two melt pond schemes and three snow redistribution configurations. The three snow redistribution configurations are bulk scheme, snwITDrag scheme and one simulation selection without snow redistribution. In both bulk and snwITDrdg snow redistribution schemes, snow can be lost to leads and open water. In the bulk scheme, snow from level ice can be lost to leads or open water. In snwITDrdg scheme, snow is distributed to different sea ice categories and the scheme also allows wind-driven snow compaction and erosion. The two melt pond schemes are TOPO scheme and LVL scheme, which differ in the distribution of melt water. The results show that Icepack can reproduce sea ice growth in the winter and spring periods of MOSAiC expedition. Icepack without snow redistribution scheme simulates excessive snow ice formation and its contribution to sea ice mass balance, resulting in thicker SIT simulation than the observation in spring. Applying snow redistribution schemes in Icepack reduces snow-ice formation while enhancing congelation rate. The bulk snow redistribution scheme improves the SIT simulation in winter and spring, while the bias is larger in simulations using the snwITDrdg scheme. During summer time, Icepack underestimates the sea ice surface albedo, resulting in an underestimation of SIT at the end of simulation. The simulations with TOPO scheme present a more reasonable melt pond evolution than the LVL scheme, resulting in a smaller bias in SIT simulation. Sensitivity analysis and parameter estimation are required to improve sea ice thickness simulation. Some earlier results using adjoint model to improve sea ice simulation will also be presented.

How to cite: Lu, Y., Zhao, J., Wang, X., and Giering, R.: Influence of Snow Redistribution and Melt Pond Schemes on Sea Ice Thickness Simulation during MOSAiC Expedition, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21072, https://doi.org/10.5194/egusphere-egu25-21072, 2025.

NP2 – Dynamical Systems Approaches to Problems in the Geosciences

EGU25-334 | ECS | Posters on site | NP2.2

A new process-based carbon cycle for the FaIR simple climate model 

Alejandro Romero-Prieto, Camilla Mathison, Piers Forster, Glen Harris, Chris Jones, Ben Booth, and Chris Smith

Simple Climate Models (SCMs) provide an efficient way to explore potential climate futures by quickly evaluating emissions and mitigation scenarios.  This efficiency enables applications beyond the capabilities of complex Earth System Models (ESMs), such as integration with integrated assessment models and reactive policy analysis. A prominent example of this type of models is the FaIR SCM, which has gained popularity in recent years and been applied in various contexts. However, the current implementation of FaIR’s carbon cycle lacks detail, as it does not resolve the carbon fluxes between different ecosystem components. This limitation reduces the model’s flexibility and prevents it from participating in carbon-focused research.

Here, we present a new simple carbon cycle model that simulates the evolution of the global carbon stocks and fluxes across the atmosphere, ocean, soil and vegetation pools. The model calibration used data from 13 ESMs participating in the 6th Coupled Model Intercomparison Project (CMIP6), including all model simulations for the Shared Socioeconomic Pathways (SSP) scenarios. We evaluate the model’s performance in emulating ESM carbon cycles and discuss the integration with the FaIR SCM. By using the calibrations to CMIP6 ESMs and sampling the uncertainty parameters in our carbon cycle model, we can obtain posterior sets that compare well with best available observations, such as the growth in land, ocean and atmospheric stocks from the annual Global Carbon Budget. This enhancement to FaIR to include a process-based carbon cycle significantly strengthens its carbon cycle capabilities, unlocking new research opportunities.

How to cite: Romero-Prieto, A., Mathison, C., Forster, P., Harris, G., Jones, C., Booth, B., and Smith, C.: A new process-based carbon cycle for the FaIR simple climate model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-334, https://doi.org/10.5194/egusphere-egu25-334, 2025.

EGU25-1288 | ECS | Orals | NP2.2

The influence of freshwater biases on AMOC stability and consequences for CMIP6 models 

Amber Boot and Henk Dijkstra

The Atlantic Meridional Overturning Circulation (AMOC) modulates global climate and has been identified as a potential tipping element that might collapse under future climate change. Such a collapse would have strong global consequences for the climate system, ecosystems and society. The IPCC AR6 report states that it is unlikely that the AMOC will collapse in the 21st century which is mostly based on CMIP6 type Earth System Model results. However, these models have strong biases that can affect AMOC stability. If these models are biased towards a too stable AMOC, they might underestimate the probability of an AMOC collapse this century. To better understand the effects of freshwater biases on AMOC stability we perform experiments with the intermediate complexity Earth System Model CLIMBER-X. By introducing both positive and negative freshwater biases in the Atlantic and Indian Ocean we can gain a better understanding on how these biases affect AMOC stability. We find that introducing fresh biases in the Indian Ocean leads to an increase in stability, whereas fresh biases in the Atlantic Ocean lead to a decrease in stability. The combined effect of the biases in the Atlantic and Indian Ocean is near linear. We project the results of CLIMBER-X onto CMIP6 model biases such that we can assess whether CMIP6 models are likely simulating a too stable or too unstable AMOC.    

How to cite: Boot, A. and Dijkstra, H.: The influence of freshwater biases on AMOC stability and consequences for CMIP6 models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1288, https://doi.org/10.5194/egusphere-egu25-1288, 2025.

EGU25-2101 | Orals | NP2.2

TSformer: A Non-autoregressive Spatial-temporal Transformers for 30-day Ocean Eddy-Resolving Forecasting 

Guosong Wang, Xinrong Wu, Zhigang Gao, Min Hou, and Mingyue Qin

Ocean forecasting is critical for various applications and is essential for understanding air-sea interactions, which contribute to mitigating the impacts of extreme events. State-of-the-art ocean numerical forecasting systems can offer lead times of up to 10 days with a spatial resolution of 10 kilometers, although they are computationally expensive. While data-driven forecasting models have demonstrated considerable potential and speed, they often primarily focus on spatial variations while neglecting temporal dynamics. This paper presents TSformer, a novel non-autoregressive spatiotemporal transformer designed for medium-range ocean eddy-resolving forecasting, enabling forecasts of up to 30 days in advance. We introduce an innovative hierarchical U-Net encoder-decoder architecture based on 3D Swin Transformer blocks, which extends the scope of local attention computation from spatial to spatiotemporal contexts to reduce accumulation errors. TSformer is trained on 28 years of homogeneous, high-dimensional 3D ocean reanalysis datasets, supplemented by three 2D remote sensing datasets for surface forcing. Based on the near-real-time operational forecast results from 2023, comparative performance assessments against in situ profiles and satellite observation data indicate that, TSformer exhibits forecast performance comparable to leading numerical ocean forecasting models while being orders of magnitude faster. Unlike autoregressive models, TSformer maintains 3D consistency in physical motion, ensuring long-term coherence and stability in extended forecasts. Furthermore, the TSformer model, which incorporates surface auxiliary observational data, effectively simulates the vertical cooling and mixing effects induced by Super Typhoon Saola.

How to cite: Wang, G., Wu, X., Gao, Z., Hou, M., and Qin, M.: TSformer: A Non-autoregressive Spatial-temporal Transformers for 30-day Ocean Eddy-Resolving Forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2101, https://doi.org/10.5194/egusphere-egu25-2101, 2025.

EGU25-2501 | Posters on site | NP2.2

A Residual Ordering of SST Koopman Spectra for the Identification of Fundamental Modes 

Paula Lorenzo Sánchez and Antonio Navarra

El Niño-Southern Oscillation (ENSO) is a prominent driver of global climate variability, with significant impacts on ecosystems and societies. While existing empirical-dynamical forecasting methods, such as Linear Inverse Models (LIMs), are limited in capturing ENSO's inherent nonlinearity, Koopman operator theory offers a framework for analyzing such complex dynamics. Recent advancements in Koopman-based methods, such as DMD-based methods, have enabled exploration of nonlinear ENSO-related modes. However, they often suffer from challenges in robustness and interpretability. Specifically, k-EDMD algorithms tend to produce a large number of modes, complicating their physical relevance and reliability. In this study, we address these limitations by employing Colbrook’s Residual EDMD (Res-EDMD) framework as a tool to classify and prioritize modes based on their residuals. This approach enables us to systematically identify robust and physically meaningful modes, distinguishing them from less reliable counterparts. Furthermore, leveraging the property that eigenfunctions of Koopman operators can generate higher-order harmonics through powers and multiplications, we introduce a methodology to detect fundamental modes and their associated harmonics. Applying this framework to tropical Pacific SST data, we demonstrate that k-EDMD, together with Res-EDMD, are capable of isolating fundamental modes of tropical SST dynamics. These fundamental modes provide insights into the system's physical evolution and facilitate the retrieval of meaningful dynamical information. By systematically identifying and interpreting the modes, we establish a pathway to overcome the limitations of conventional Koopman-based methods, thereby enhancing their applicability for studying and forecasting complex climatic systems like ENSO. This study underscores the potential of Res-EDMD to refine mode selection in Koopman spectral analysis, paving the way for robust, physically interpretable insights into tropical SST variability.

How to cite: Lorenzo Sánchez, P. and Navarra, A.: A Residual Ordering of SST Koopman Spectra for the Identification of Fundamental Modes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2501, https://doi.org/10.5194/egusphere-egu25-2501, 2025.

EGU25-2814 | ECS | Orals | NP2.2

Ensemble simulation of the AMOC collapse in a conceptual climate model 

Dániel Jánosi, Ferenc Divinszki, Reyk Börner, and Mátyás Herein

The Atlantic Meridional Overturning Circulation (AMOC) is a mechanism of great importance, as its possible collapse would constitute a dramatic response to Earth’s changing climate. The AMOC is particularly important for Northern Europe, as it plays a central role in regulating the region’s climate, and a slowdown or collapse would lead to a significant cooling of the region. This critical transition has been the subject of many studies over the years, both from the aspects of climate modeling and dynamical systems theory. In the context of the latter, climate change is nothing but a complex, chaotic-like system, which possesses a time-dependent parameter, in the shape of e.g. the growing CO2 concentration. It has been known for some time now, that such systems not only have a chaotic attractor, but one which is also time-dependent, a so-called snapshot attractor. Such objects, and thus the systems they describe, can only be faithfully represented by statistics over an ensemble of trajectories, a single one does not suffice. We perform such ensemble simulations on a conceptual climate model of the AMOC, constructed by coupling the Lorenz84 and the Stommel box models. We find that the difference between the ensemble members in the point when the collapse occurs can be up to hundreds of years, and that some trajectories can even survive with the AMOC remaining in the “on” state.  This highlights the fact that that a single trajectory is unreliable, however, with the proper ensemble statistics (e.g. standard deviations, time-dependent Lyapunov exponents, etc), a probabilistic description of the collapse can be given.

How to cite: Jánosi, D., Divinszki, F., Börner, R., and Herein, M.: Ensemble simulation of the AMOC collapse in a conceptual climate model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2814, https://doi.org/10.5194/egusphere-egu25-2814, 2025.

EGU25-3266 | ECS | Orals | NP2.2

Non-Equilibrium Thermodynamics and Climate Predictability: Investigating Entropy Production and Frenesy 

Roberta Benincasa, Jeffrey B. Weiss, Danni Du, Gregory S. Duane, and Nadia Pinardi

Assessing climate predictability remains a central challenge in modeling and forecasting the climate system. Approaches from nonequilibrium statistical mechanics, particularly stochastic thermodynamics, have provided insights into non-equilibrium properties of stochastic models, which have proven useful in representing patterns of climate variability. In this work, we investigate the potential of entropy production and frenesy as tools for quantifying the predictability of non-equilibrium fluctuations in the climate system. Entropy production, a measure of the irreversibility of the system’s dynamics, is explored as an intrinsic indicator of predictability and its possible connections to the Anomaly Correlation Coefficient (ACC). Frenesy, a lesser-known quantity derived from active matter studies that captures kinetic fluctuations and dynamical activity, is assessed for its potential role in explaining non-equilibrium processes within the climate system. Thus, we aim to better understand the relationships between these thermodynamic quantities and climate oscillations, such as the El Niño-Southern Oscillation and the Madden-Julian Oscillation, with the ultimate goal of defining a new measure of climate predictability and better comprehending non-equilibrium processes in the ocean and the atmosphere.

How to cite: Benincasa, R., Weiss, J. B., Du, D., Duane, G. S., and Pinardi, N.: Non-Equilibrium Thermodynamics and Climate Predictability: Investigating Entropy Production and Frenesy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3266, https://doi.org/10.5194/egusphere-egu25-3266, 2025.

EGU25-3480 | ECS | Posters on site | NP2.2

Causal analysis of time series data for modeling nonlinear phenomena 

Kazuki Kohyama, Rin Irie, and Masaki Hisada

In typhoon forecasting, air-only and coupled air-sea models have similar accuracy in predicting typhoon trajectories. However, air-sea interactions must be considered to accurately forecast typhoon intensity [1]. Although coupling between multiple modules, including turbulence, waves, ecosystem, and chemistry, has been suggested to improve forecast accuracy, the modules and their individual model equations for typhoon forecasting are still determined empirically. Accurate modeling of the interactions between phenomena across multiple modules is an essential determinant of simulation accuracy. To determine critical factors within each module, parameterizations should be determined quantitatively, not empirically. However, it is challenging to impose preconditions on models that accurately capture the many complex interactions between air and sea.

In this study, we propose a modeling method to identify these critical factors using a causal analysis based on information theory. The causality of typical causal network models depends on the precondition network shape, but by using information theory, it is possible to extract causality comprehensively without preconditions. This allows for a quantitative assessment of causality without making the assumptions necessary for causal networks, such as Bayesian networks. In the proposed method, the information flux T, also known as transfer entropy, is defined as the difference in the Shannon entropy for multi-elements Q over two timesteps tn and tn+1 [2], as follows

TJI = H(Qjn+1Q≠in ) − H(Qjn+1Qn),

= ∑i,j p(in+1,in,jn) log p(in+1in,jn) / p(in+1in),

where H(Q) = Σ p(q) log p(q) is Shannon entropy, and we define Q as containing two elements Q = (I,J). Information flux quantifies the causality and amount of information flow between two time series. The magnitude of T corresponds to the parameter value indicating the interactions within and between the models. For example, recently, this method of quantifying causality was also applied to turbulence [3], which is one of the most chaotic phenomena, and used to clarify the causality of interactions between scales in the transport of scales in developed turbulence [4]. As a first step, we apply this method to a simplified non-linear model, and try to reconstruct its original model equation for test cases of the Lotka-Volterra model and the Lorenz model. For combinations of time series data for multiple variables generated by the models as multi-dimensional ordinary differential equations, we calculated the information flux according to the equation to extract the causal relationships of combinations with high T values. Then, by selectively rebuilding the model with only the variables of the elements that cause a high Tcause→effect value as the basis of the model function, the cost of parameter optimization is reduced, and the optimal parameter values are determined by fitting with the original time series data. In the presentation, we will discuss possibilities of the proposed method and its potential applications in climate simulations.

 

References
[1] L. R. Schade and K. A. Emanuel, J. Atmos. Sci. 56, pp. 642–651 (1999).
[2] T. Schreiber, Phys. Rev. Lett. 85, pp. 461–464 (2000).
[3] A. Lozano-Durán and G. Arranz, Phys. Rev. Res. 4, 023195 (2022).
[4] R. Araki, A. Vela-Martín, and A. Lozano-Durán, J. Phys.: Conf. Ser. 2753, 012001 (2024).

How to cite: Kohyama, K., Irie, R., and Hisada, M.: Causal analysis of time series data for modeling nonlinear phenomena, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3480, https://doi.org/10.5194/egusphere-egu25-3480, 2025.

EGU25-6571 | Orals | NP2.2

Challenging the hierarchy: what could a pluralist ecosystem of climate modelling strategies look like? 

Erica Thompson, Marina Baldissera Pacchetti, and Julie Jebeile
The predominant strategy of climate modelling is to continually increase resolution and complexity of general circulation models (GCMs). At present, there are calls to double down on this strategy and invest a lot more financial and computational resource into GCM resolution and complexity, with the assumption that this will improve the usefulness of climate predictions to support climate adaptation decision making.
We argue that this is not the best use of scientific effort.  Because there are many different kinds of questions encompassed within climate decision making - involving different individuals, communities and organisations with plural value systems - many different climate modelling strategies are needed which have different methodological aims and do not necessarily form a simple linear “hierarchy”, but can still learn from and complement each other.  We contrast the strengths and weaknesses of approaches such as GCMs, machine learning methods, EMICs, toy models, and narrative or storyline approaches as well as physics-informed models such as IAMs, ecosystem models and climate fiction.
We outline some ideas for what a (more) pluralist ecosystem of climate modelling strategies would look like, and how it could more effectively answer adaptation decision questions.

How to cite: Thompson, E., Baldissera Pacchetti, M., and Jebeile, J.: Challenging the hierarchy: what could a pluralist ecosystem of climate modelling strategies look like?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6571, https://doi.org/10.5194/egusphere-egu25-6571, 2025.

EGU25-6658 | ECS | Orals | NP2.2

Dealing with bugs is part of climate modeling 

Ulrike Proske

Numerical models are not just numerical representations of physical phenomena. They are also software files written by humans. As such they contain unintended coding errors, termed bugs. While the size of climate model code and human imperfection suggest that these are frequently present in climate models (Pipitone and Easterbrook, 2012), bugs are seldom acknowledged in the literature. However, missing understanding of model bugs hinders our understanding of model results as well as our ability to improve modeling workflows.

With a case study of the ICON general circulation model (GCM), I elucidate the practices and considerations around model debugging. Specifically, I give examples for bugs detected in that GCM's development and report on qualitative in-depth interviews I conducted with 11 model developers (domain scientists and scientific programmers). The interviews show that dealing with bugs is not a standardised process. While the technical testing of ICON code developments is highly standardised, and for example the assignment of responsibility is standardised implicitly, the scientific testing resists standardisation. The missing standardisation makes dealing with bugs a laborious process that takes time and effort and where human influence is common.

While this study focusses on the meaning of bugs for GCMs, similar considerations may be at play for models from different rugs of the model hierarchy. Where they differ, the model hierarchy may offer a way to more systematically detect and fix bugs in models of any rug.

 

 

Pipitone, J. and Easterbrook, S.: Assessing climate model software quality: a defect density analysis of three models, Geosci. Model Dev., 5, 1009–1022, https://doi.org/10.5194/gmd-5-1009-2012, 2012.

How to cite: Proske, U.: Dealing with bugs is part of climate modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6658, https://doi.org/10.5194/egusphere-egu25-6658, 2025.

EGU25-9070 | ECS | Orals | NP2.2

Physics-aware kernel Koopman operator estimation for consistent nonlinear mode decomposition 

Nathan Mankovich and Gustau Camps-Valls

Nonlinear dynamical systems are ubiquitous across scientific disciplines, yet their analysis and predictive modeling remain challenging due to their inherent complexity. Koopman operator estimation and Koopman mode decomposition are common tools for emulating and extracting modes of variability from such systems. In this work, we propose a novel method for Koopman operator estimation called the Physics-Aware Koopman Operator (PAKO). Our approach is tailored for physical consistency by introducing a regularization term based on the Hilbert-Schmidt Independence Criterion (HSIC) to enforce independence between predictions and sensitive or protected physical variables. In addition to Koopman operator estimation, we extract Koopman modes and eigenvalues through a Koopman mode decomposition. We validate PAKO on the ClimateBench dataset, demonstrating superior accuracy, robustness, and interpretability for estimating the internal variability of climate systems. Our results showcase the potential of PAKO for advancing Koopman operator estimation of complex nonlinear dynamical systems.

How to cite: Mankovich, N. and Camps-Valls, G.: Physics-aware kernel Koopman operator estimation for consistent nonlinear mode decomposition, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9070, https://doi.org/10.5194/egusphere-egu25-9070, 2025.

EGU25-9917 | ECS | Orals | NP2.2 | Highlight

An unsupervised method for extracting coherent spatiotemporal patterns in multi-scale data 

Karl Lapo, Peter Yatsyshin, Brigitta Goger, Sara Ichinaga, and J. Nathan Kutz

The unsupervised and principled diagnosis of multi-scale data is a fundamental obstacle in earth sciences. Here we explicitly define multi-scale data as being characterized by spatiotemporal processes (i.e. processes acting along time and space simultaneously) with process scales acting across orders of magnitude, non-stationarity, and/or invariances such as translation and rotation. Existing methods, such as traditional analytic approaches, data-driven modeling like Dynamic Mode Decomposition (DMD), and even deep learning, are not well-suited to diagnosing multi-scale data, usually requiring supervised strategies such as human intervention, extensive tuning, or selection of ideal time periods.

We present the multi-resolution Coherent Spatio-Temporal Scale Separation (mrCOSTS), a data-driven method capable of overcoming the challenges of multi-scale data. It is a hierarchical variant of Dynamic Mode Decomposition (DMD) that enables the unsupervised extraction of spatiotemporal features in multi-scale data. It operates by decomposing the data into bands of temporal frequencies associated with coherent spatial modes. The method requires no training and functions with little to no hyperparameter tuning by instead taking advantage of the hierarchical nature of multi-scale systems.

We demonstrate mrCOSTS on multi-scale data from a range of disciplines and scales: 1) sea surface temperature of the El-Nino Southern Oscillation (ENSO), 2) Antartic sea ice concentration, and 3) directly evaluating a numerical weather model against LIDAR observations of wind speed. In each example we demonstrate how mrCOSTS can be used to gain insights into the underlying dynamics of each system, revealing missing components in the description of each system's variability, diagnosing extreme events, and provide a pathway forward for building better physical representations in models.

Using mrCOSTS, we show that ENSO is the result of 6 coherent spatio-temporal bands and use these results to explain the difference in intensity and spatial pattern of extreme 2015-2016 ENSO event relative to other extreme ENSO events. In the second example, we show that the dynamics of Antarctic sea ice concentration were found to have a negligible interannual component until 2012 when a long-term decline initiated and interannual dynamics at a decadal-scale started contributing. The large decline in sea ice concentration between 2014-2017 was almost entirely the result of the new interannual dynamics while the recent record low sea ice concentrations had a strong climate change signal. Finally, we demonstrate how mrCOSTS enables the evaluation of models directly against spatially-explicit observations. We evaluated an eddy-resolving numerical model against LIDAR observations of wind speed. The scale-aware model evaluation allowed us to easily reveal that errors at the largest scales dominated the system despite the agreement of lower order statistical moments. In each case using mrCOSTS we trivially retrieved complex dynamics that were previously difficult to resolve while additionally extracting previously unknown patterns or complexities of systems characterized by multi-scale processes.

How to cite: Lapo, K., Yatsyshin, P., Goger, B., Ichinaga, S., and Kutz, J. N.: An unsupervised method for extracting coherent spatiotemporal patterns in multi-scale data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9917, https://doi.org/10.5194/egusphere-egu25-9917, 2025.

Connecting the different levels of the hierarchy of complexity in which climate models operate, and comparing the assumptions that apply at each level, has led to much progress in climate science. A particularly notable success was Klaus Hasselmann’s use of Brownian motion to inspire his linear Markovian stochastic energy balance model (EBM), the history of which was recently summarised by Watkins [2024]. Another informative, but lateral, connection and comparison is that between either studying climate through the lens of stochastic physical models or doing so via statistical methods. This presentation showcases how comparing these approaches can sometimes surprise us.

It has been asserted that because the Hasselmann stochastic EBM has a mean-reverting term due to feedbacks, this property must also be detected in global mean temperature time series by statistical models such as the well-known Box-Jenkins ARIMA family. Conversely its absence has been taken as an indication of fundamental difficulties with anthropogenic driving. By fitting Hasselmann models, with and without anthropogenic driving, to an ARFIMA model with automatically selected parameters we show that in fact the absence of a prominent autoregressive term has precisely the opposite meaning, and is, rather, a clear indication of strong driving.

We will also report preliminary findings about the extent to which the presence of long range memory due to the multiple time scales present in the coupled ocean-atmosphere can affect the above conclusions, updating  the work summarised by Watkins et al [2024]. We thank Nick Moloney for many insightful suggestions.

Watkins, N. W., "Brownian motion as a mathematical superstructure to organise the science of climate and weather", In Foundational Papers in Complexity Science, Volume 3, pp. 1481–1510. Edited by David C. Krakauer. Santa Fe, NM: SFI Press. DOI: 10.37911/9781947864542.51 (2024).

Watkins, N. W., R. Calel, S. C. Chapman, A. Chechkin, R. Klages and D. Stainforth,   The Challenge of Non-Markovian Energy Balance Models in Climate.  Chaos. 34, 072105 . DOI:10.1063/5.0187815 (2024).

 

How to cite: Watkins, N. W. and Stainforth, D.:  Comparing the views of the driven climate system through the lenses of statistical time series analysis  and stochastic EBMs: Apparent absence of mean reversion can be evidence of anthropogenic driving., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12353, https://doi.org/10.5194/egusphere-egu25-12353, 2025.

EGU25-12960 | ECS | Orals | NP2.2

Data-driven Discovery of Predictive Spatiotemporal Patterns leading to Tropical Cyclogenesis 

Frederick Iat-Hin Tam, Tom Beucler, and James Ruppert

The early intensification (genesis) of tropical cyclones (TCs) is challenging to predict accurately in operational settings. The difficulty in predicting TC genesis stems from an insufficient understanding of the thermodynamic-kinematic characteristics involved in the multiscale interaction between clouds and TC circulations leading to genesis. Cloud-radiative feedback (CRF) has been shown to play a critical role in accelerating intensification during genesis by initiating secondary circulations that drive moisture and momentum convergence. However, it is still challenging to identify the exact pattern in radiation that could benefit genesis the most. Traditional diagnostic approaches to isolate CRF, such as the Sawyer-Eliassen Equation, require steady-state, axisymmetric thermal forcing. As such, these diagnostics methods are likely suboptimal in studying the response of weak TCs to intermittent, spatially asymmetric thermal forcing. 

 

This presentation utilizes novel data-driven methodologies to identify complex three-dimensional radiative patterns and approximate the thermodynamic-kinematic feedback between such patterns and early TC intensification. Specifically, we tasked a stochastic Variational Encoder-Decoder (VED) framework to discover different predictive patterns in radiative heating and quantify how these patterns affect early TC intensification. Applying the proposed framework to ensemble WRF simulations of Typhoon Haiyan (2013), longwave radiation anomalies in the downshear quadrants of Haiyan are shown to be particularly relevant to the early intensification of that TC. The extracted patterns provide new insights into how deep convective and shallow clouds should distribute spatially to best accelerate genesis. Apart from analyzing the extracted pattern, the stochastic nature of the proposed ML architecture brings additional insights into the radiatively-driven TC genesis research problem. We can use uncertainty in the prediction of intensification rates to track the time evolution of the relevance of radiation in tropical cyclone intensification. Furthermore, the uncertainty in the extracted pattern allows us to pinpoint trustworthy regions in the discovered predictive patterns for scientific interpretation.

 

Our study underscores the potential use of data-driven methodologies to quantify the impact of asymmetric radiative forcing on early TC formation without relying on axisymmetric or steady-state assumptions. The successful application of VED in this presentation reveals a promising way to use data-driven methods to uncover new knowledge in weather dynamics.

Reference:

Iat-Hin Tam, F., Beucler, T., & Ruppert, J. H., Jr. (2024). Identifying three-dimensional radiative patterns associated with early tropical cyclone intensification. Journal of Advances in Modeling Earth Systems, 16, e2024MS004401. https://doi.org/10.1029/2024MS004401

 

How to cite: Tam, F. I.-H., Beucler, T., and Ruppert, J.: Data-driven Discovery of Predictive Spatiotemporal Patterns leading to Tropical Cyclogenesis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12960, https://doi.org/10.5194/egusphere-egu25-12960, 2025.

EGU25-14237 | Orals | NP2.2

The Role of Internal Climate Variability in Noise-Shaped Hysteresis Cycles of the AMOC Under Rising CO2 Forcing 

Susanna Corti, Matteo Cini, Giuseppe Zappa, and Francesco Ragone

The Atlantic Meridional Overturning Circulation (AMOC), is a key tipping element of the climate system. A tipping point typically results from the interplay between external forcing (such as increased GHGs concentration or freshwater input) and the intrinsic internal variability of the system. While most studies mainly focus on identifying a critical forcing threshold (i.e. the minimal CO2 concentration or anomaly freshwater input needed for the collapse), the role of the internal climate variability remains less explored. Investigating the role of the internal variability requires performing large ensemble simulations which are  typically unfeasible with state-of-the-art models and traditional approaches. In our study, using an intermediate complexity model (PlaSIM-LSG, T21), once we assessed noise-induced collapse with a rare event algorithm, we investigated at which extent climate variability affects AMOC stability when CO2 forcing is applied. Traditionally, the AMOC stability landscape is investigated using single-realization hysteresis diagrams, driven by freshwater input in the North Atlantic. However, the effects of gradual CO2 forcing and, in particular, the impact of internal climate variability on the timing of AMOC tipping points have been less studied.  We conducted three independent hysteresis simulations, applying a slow CO2 ramp-up and ramp-down (0.2 ppm/year). Our findings reveal that internal variability strongly affects the timing of the AMOC tipping and the shape of the hysteresis cycle. In one simulation, we observed a reversed cycle, where the AMOC recovers at higher CO2 levels than at collapse. While statistical Early Warning Signals (EWS) provide some indication of approaching tipping points, the internal variability considerably reduces their predictability and introduces false positives. This suggests that AMOC behavior, when internal climate variability is considered, can differ significantly from characteristics of simpler models, and that caution is needed when interpreting results from a single-experiment realization. Moreover, the role of internal climate variability suggests that a probabilistic approach is necessary to define AMOC’s “safe operating space”, since it might not be possible to define a single critical CO2 threshold to prevent AMOC collapse.

How to cite: Corti, S., Cini, M., Zappa, G., and Ragone, F.: The Role of Internal Climate Variability in Noise-Shaped Hysteresis Cycles of the AMOC Under Rising CO2 Forcing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14237, https://doi.org/10.5194/egusphere-egu25-14237, 2025.

EGU25-14642 | ECS | Posters on site | NP2.2

Using Deep Learning to Identify Initial Error Sensitivity for Interpretable ENSO Forecasts 

Kinya Toride, Matthew Newman, Andrew Hoell, Antonietta Capotondi, Jakob Schlör, and Dillon Amaya

We introduce an interpretable-by-design method, optimized model-analog, that integrates deep learning with model-analog forecasting which generates forecasts from similar initial climate states in a repository of model simulations. This hybrid framework employs a convolutional neural network to estimate state-dependent weights to identify initial analog states that lead to shadowing target trajectories. The advantage of our method lies in its inherent interpretability, offering insights into initial-error-sensitive regions through estimated weights and the ability to trace the physically-based evolution of the system through analog forecasting. We evaluate our approach using the Community Earth System Model Version 2 Large Ensemble to forecast the El Niño-Southern Oscillation (ENSO) on a seasonal-to-annual time scale. Results show a 10% improvement in forecasting equatorial Pacific sea surface temperature anomalies at 9-12 months leads compared to the unweighted model-analog technique. Furthermore, our model demonstrates improvements in boreal winter and spring initialization when evaluated against a reanalysis dataset. Our approach reveals state-dependent regional sensitivity linked to various seasonally varying physical processes, including the Pacific Meridional Modes, equatorial recharge oscillator, and stochastic wind forcing. Additionally, forecasts of El Niño and La Niña are sensitive to different initial states: El Niño forecasts are more sensitive to initial error in tropical Pacific sea surface temperature in boreal winter, while La Niña forecasts are more sensitive to initial error in tropical Pacific zonal wind stress in boreal summer. This approach has broad implications for forecasting diverse climate phenomena, including regional temperature and precipitation, which are challenging for the model-analog approach alone.

How to cite: Toride, K., Newman, M., Hoell, A., Capotondi, A., Schlör, J., and Amaya, D.: Using Deep Learning to Identify Initial Error Sensitivity for Interpretable ENSO Forecasts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14642, https://doi.org/10.5194/egusphere-egu25-14642, 2025.

EGU25-15878 | Posters on site | NP2.2

Spatiotemporal Similarity-Based Approach for Analyzing the Relationship Between Sea Fog Occurrence and Sea Level Pressure Distributions 

Sung-Hwan Park, Hojin Kim, Ki-Young Heo, and Nam-Hoon Kim

This study presents a novel methodology for analyzing the relationship between sea level pressure (SLP) distributions and sea fog occurrences, focusing on a spatiotemporal similarity-based approach. Using SLP data from 2001 to 2019 and visibility observations from Baengnyeong Island (BYI), Yellow Sea, the proposed framework quantifies the connection between atmospheric pressure patterns and sea fog formation. The methodology integrates three key components: defining temporal and spatial domains, calculating weighted similarities, and validating the results using sea fog occurrence data. The temporal domain was set to a 7-hour period, determined by analyzing visibility trends prior to sea fog events. This period captures the critical atmospheric changes leading to fog formation. Spatially, a 2D weighted map was constructed using Pearson correlation coefficients between SLP variations at BYI and other locations in the study area. This weighting emphasizes regions with strong correlations, ensuring the analysis focuses on areas most relevant to sea fog dynamics. The Spatiotemporal Similarity Measure (STSM) method was then applied to compare reference SLP maps from 2017–2019 with historical SLP data from 2001–2015. By identifying historical cases with high similarity to reference conditions, the study examined the likelihood of sea fog occurrences under similar atmospheric setups. These similarities were categorized into thresholds, and their connection to sea fog events was evaluated using Probability of Detection (POD) and False Alarm Ratio (FAR) metrics. The results demonstrate that higher SLP similarity corresponds to increased POD and decreased FAR, validating the effectiveness of the STSM method. This approach highlights the role of recurring SLP patterns in sea fog formation and underscores the utility of historical data in improving sea fog forecasting.

How to cite: Park, S.-H., Kim, H., Heo, K.-Y., and Kim, N.-H.: Spatiotemporal Similarity-Based Approach for Analyzing the Relationship Between Sea Fog Occurrence and Sea Level Pressure Distributions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15878, https://doi.org/10.5194/egusphere-egu25-15878, 2025.

EGU25-16465 | ECS | Posters on site | NP2.2

Simplifying Earth System Projections: Mimicking ESM Results with a Diffusion Model 

Edward Gow-Smith, Roberta Benincasa, Marco M. De Carlo, Evgeny Ivanov, Simone Norberti, and Will Chapman

Ensemble simulations using Earth System Models (ESMs) have historically been used to gain insights into future climate scenarios. However, they present notable disadvantages, particularly their long computing times and the high technical threshold required for accessibility. The recent rise of data-driven approaches offers a promising alternative, making long-term climate projections more efficient, accessible to policymakers and regional planners, and scalable for specific regions.

During the Winter School “Data-Driven Modeling and Predictions of the Earth System,” we compared the results of a simple diffusion model with the ensemble results from the CESMv.2.1.5 Large Ensemble from model year 2015 to 2090. The diffusion model, trained on CESM data, uses only CO₂ concentration and the month of the year as context channels to predict spatially-resolved, monthly averaged air temperature, precipitation, and atmospheric pressure on a global scale. The project aimed to demonstrate how effectively the diffusion model simulates global and regional variability and long-term trends in these atmospheric variables compared to the ESM. Particular attention was given to its representation of the El Niño–Southern Oscillation (ENSO) region. Additionally, a bias correction was applied to the diffusion model results against the ESM to evaluate distortions in trends and variability.

The study concluded that even a simple diffusion model has significant potential for predicting meteorological parameters based solely on projected greenhouse gas emissions and the time of year. However, its performance weakened near the poles in reproducing ESM results, highlighting the importance of incorporating additional geographic variables (e.g., grid cell size) during training. Despite these limitations, combining the strengths of coupled ESMs with diffusion models can leverage the physical accuracy of ESM outputs and the computational efficiency and adaptability of diffusion models, offering a more comprehensive understanding of Earth system dynamics.

How to cite: Gow-Smith, E., Benincasa, R., De Carlo, M. M., Ivanov, E., Norberti, S., and Chapman, W.: Simplifying Earth System Projections: Mimicking ESM Results with a Diffusion Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16465, https://doi.org/10.5194/egusphere-egu25-16465, 2025.

EGU25-17680 | Orals | NP2.2

Climate-carbon cycle modelling hierarchy 

Chris Jones

Much climate science relies on numerical modelling to both understand the processes of the Earth system and to make predictions or projections of how it may change in the future. International climate policy relies on the outcomes of these models to make decisions which will affect the lives and livelihoods of billions of people – so it is vital that they are well understood and their use is based on robust understanding of what they can (and also what they cannot) tell us.

Spatially resolved General Circulation Models (GCMs) have evolved over recent decades in both their spatial resolution (allowing finer detail to be studied) and their process complexity (including but not limited to biogeochemistry and feedbacks between climate and ecosystems). This expansion of their capability makes them more useful and relevant than ever, but they are extremely slow to run on even the worlds most powerful super computers. Conversely very simple models exist which can be run thousands (or millions) of times, but do not include the full detail of the GCMs. Finally there are models of intermediate complexity which sit between these extremes and also make valuable contributions through differing combinations of comprehensiveness and computational efficiency.

All classes of models have something to offer – it is important to understand their strengths and weakness and to choose the most suitable tool for the job. Moreover, use of these models together can be very powerful. For example IPCC reports tend to draw firstly on complex GCMs but then through thorough calibration processes propagate their information to larger numbers of scenarios using simplified climate emulators.

In this talk I will briefly outline how this mode of use of the full modelling hierarchy has developed in the field of carbon cycle feedbacks and in quantifying the remaining carbon budget – which allows detailed planning of climate mitigation policy aligned with the goals of the Paris Agreement. I will show the development of our understanding of climate-carbon cycle feedbacks from complex models and how these have been used first to determine a simple relationship between cumulative CO2 emissions and global warming (so called TCRE: transient climate response to carbon emissions), and then how simple models have been used in conjunction with complex models to explore the processes behind this relationship and begin to allow propagation of observational constraints.

I will end by outlining emerging knowledge on the strengths and weakness of each class of model (e.g. how simple is too simple?) and identifying research gaps for moving forward.

How to cite: Jones, C.: Climate-carbon cycle modelling hierarchy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17680, https://doi.org/10.5194/egusphere-egu25-17680, 2025.

There is a long history of global climate model (GCM) studies of the response of the Atlantic Meridional Overturning Circulation to changing greenhouse gases (GHGs). Alongside this is an almost separate branch of the literature studying the AMOC’s response to fresh water input (‘hosing’) with fixed GHGs, focusing on the potential for ‘tipping’ behaviour. Some common model responses are observed among models (e.g. in GHG experiments an initial AMOC weakening associated with warming of the subsurface North Atlantic), but also considerable diversity, especially in the long-term response following stabilisation of GHG concentrations or hosing.

In recent years a few studies have emerged that use in-depth analysis frameworks to give insight into individual model responses, or into the differences between model responses. However the two branches of the literature (GHG and hosing response) have remained largely independent, and there is an increasing recognition that in real-world climate change the ‘smooth’ response to GHGs and potential abrupt ‘tipping’ responses need to be considered together. Given the diversity of model responses it will be valuable to establish whether there is a simple model framework that captures the potential mechanisms of response to GHGs and hosing that have been identified in GCMs. Such a model can then be used to characterise the types of qualitative behaviour that are possible in the more relevant scenario of tipping in a warming climate.   

We present a simple box model of thermally- and haline-driven AMOC change that aims to capture in as simple a form as possible many of the mechanisms of the AMOC responses to GHGs and hosing that have been identified in the literature. To develop this from an earlier model (that captured purely the hosing response), it was found necessary to add both a simple representation of basin-scale energy and water balances, and a simple representation of varying stratification in the sub-polar North Atlantic, increasing the dynamical degrees of freedom of the model.

We show that the model captures a wide range of behaviours seen in GCM experiments, and use it to identify circumstances in which AMOC tipping may be possible without requiring unrealistic additional water input from the Greenland Ice Sheet.

How to cite: Wood, R.: Towards a unified understanding of AMOC changes under warming and fresh water forcing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17881, https://doi.org/10.5194/egusphere-egu25-17881, 2025.

EGU25-19443 | ECS | Orals | NP2.2

Linking response to forcing to natural variability using a Koopman operator formalism 

John Moroney, Valerio Lucarini, and Niccolò Zagli

Response theory has been shown to be a powerful tool in determining the impact of external forcing on the earth’s climate. High sensitivity to perturbations and the slow decay of response functions is associated with critical behaviour and tipping points. Despite the nonlinear nature of the climate dynamics, a generalisation of the fluctuation-dissipation theorem provides a direct connection between these response functions and the natural variability of the system. We show how response functions for a complex dynamical system may be written as a sum of terms that depend on the eigenvalues and eigenfunctions of the Koopman operator of the system, each term corresponding to a mode of variability. We demonstrate in a number of low-dimensional examples how extended dynamic mode decomposition may be used to accurately compute response and correlation functions of various observables, given only a set of snapshot data.

How to cite: Moroney, J., Lucarini, V., and Zagli, N.: Linking response to forcing to natural variability using a Koopman operator formalism, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19443, https://doi.org/10.5194/egusphere-egu25-19443, 2025.

EGU25-19722 | Orals | NP2.2

A stable hothouse triggered by a tipping mechanism 

Erik Chavez, Michael Ghil, and Jan Rombouts

The climate system is nonlinear and affected by both natural variability and several types of forcing. The impact of anthropogenic forcing and environmental change on several of the system's nonlinear processes has led to considerable concern about the tipping of regional subsystems (e.g. Lenton, 2016), due to their potentially irreversible consequences. On the global level, these nonlinear effects have been shown to give rise to bistability (Stommel, 1961} and chaotic behavior (Lorenz, 1963) in the system's past (e.g., Boers et al, 2022), as well as having been proposed conceptually as due to occur in its future, too (e.g., Steffen et al, 2018). However, specific mechanisms for a sudden tipping to an alternate stable “hothouse”, several degrees warmer than the present climate, have not been explored so far to a satisfactory extent with ESM-based studies using aqua planets (e.g., Ferreira et al 2011, Popp et al, 2016).

   Here we show that a highly simplified energy balance model (EBM) of globally averaged temperature T representing the radiative budget, coupled with a three box-type model of global carbon dynamics, does exhibit such an alternate stable hothouse climate with T higher by roughly 10 °C than the present. This TCV model also captures quite accurately the fluxes of carbon between the separate reservoirs of the coupled atmosphere-land-ocean system, when compared with observations and with simulations by high-end models. The model includes two regional mechanisms, that trigger a global tipping to such a hothouse. The two regional mechanisms are (i) the decrease of terrestrial albedo due to the darkening of ice sheets by pervasive glacial micro algal growth (e.g., Williamson et al, 2020) not included in ESMs to date; and (ii) the limits of vegetation adapting to increased environmental stress and, hence, the reduction of its carbon absorbtion (e.g., Hammond, 2022).

    These findings and the mechanistic understanding of the processes leading to a global tipping can contribute to a fruitful dialogue between the conceptual-model and ESM communities. Such a dialogue can greatly enhance our understanding of the climate system’s potential for global tipping in response to anthropogenic greenhouse gas emissions.  

How to cite: Chavez, E., Ghil, M., and Rombouts, J.: A stable hothouse triggered by a tipping mechanism, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19722, https://doi.org/10.5194/egusphere-egu25-19722, 2025.

EGU25-20182 | Orals | NP2.2

Morphological cellular analysis of Pockets of Open Cells on Marine 

Jan Haerter and Diana Monroy

More of Earth’s surface is covered by Stratocumulus clouds (Sc) than by any other cloud
type making them extremely important for Earth’s energy balance, mostly due to reflection of
solar radiation. However, representing Sc and their radiative impact is one of the largest chal-
lenges for global climate models because these cannot resolve the length scales of the processes
involve in its formation and evolution. For this reason, Sc clouds represent a large uncertainty
for climate projections [1].
The challenge becomes more intricate due to the organizational complexity that Sc clouds
present in a broad range of spatial scales. In particular, Sc fields over the oceans display
characteristic mesoscale patterns that can present both organized and unorganized structures.
Between these morphological types, cellular convection receives particular attention given than
cloud decks self-organize into honeycomb-like hexagonal patterns composed by closed and
open convective cells fields.
The purpose of this project is to analyze satellite images of a particular tendency of Sc to orga-
nize into spatially compact, cellular-patterned, low-reflectivity regions of open cells embedded
in closed cellular cloud fields called as pockets of open cells (POCs) [2].
We aim to propose a segmentation, cell tracking and quantitative analysis of cell shape and
behavior changes in closed and open cell fields, in particular the interaction of both cells when
POCs are formed. A statistical analysis of different POCs will be carried to describe the time
and spatial contributions of cell shape changes, transitions and rearrangements in the evolution
of cellular patterns on Sc clouds considering the local dynamics between individual cells.
We hypothesize that the interaction between cold pools that are formed when open cells pre-
cipitate triggers a rapid dynamics on open cells fields. For its part, closed cells fields present
steady morphology until perturbations are formed triggering the formation of POCs.

How to cite: Haerter, J. and Monroy, D.: Morphological cellular analysis of Pockets of Open Cells on Marine, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20182, https://doi.org/10.5194/egusphere-egu25-20182, 2025.

EGU25-20523 | Posters on site | NP2.2

Seasonal Forecasts with Transformers methods 

Antonio Navarra

Transformer-based approaches to seasonal forecasting have emerged as powerful tools in predicting climate patterns by leveraging deep learning techniques. These models, initially designed for natural language processing, excel in capturing long-range dependencies and complex temporal patterns, making them suitable for climate data characterized by intricate temporal relationships. In seasonal forecasting, transformers can process sequential data such as surface temperature and SST, learning from historical patterns to predict future seasonal variations.

A crucial enhancement to this approach is the exploitation of spatial coherence, which is often captured by variance modes. Variance modes, such as those derived from empirical orthogonal functions (EOFs), identify dominant spatial patterns in climate data, encapsulating the spatial correlations across different regions. By integrating these modes into transformer models, it becomes possible to enhance the model’s understanding of spatial dependencies, leading to more accurate and coherent seasonal forecasts.
Furthermore, the model allows to focus on the predictability of time means, from monthly to seasonal, and also on specific sectors of the variabilith as they are identified by EOFs. This approach aligns with practical forecasting needs, where average conditions over extended periods are often more relevant than short-term fluctuations. By combining transformers, spatial coherence, and time-averaged data, this method holds significant promise for advancing seasonal climate forecasting.

How to cite: Navarra, A.: Seasonal Forecasts with Transformers methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20523, https://doi.org/10.5194/egusphere-egu25-20523, 2025.

The influence of structural errors in general circulation models (GCMs) — stemming from missing physics, imperfect parameterizations of subgrid-scale processes, limited resolution, and numerical inaccuracies — results in systematic biases across various components of the Earth system.

 

In this talk, we develop an approach to correct biases in the atmospheric component of the Community Earth System Model (CESM) using convolutional neural networks (CNNs) to create a corrective model parameterization for online bias reduction. By learning to predict systematic nudging increments derived from a linear relaxation towards the ERA5 reanalysis, our method dynamically adjusts the model state, significantly outperforming traditional corrections based on climatological increments alone. Our results demonstrate substantial improvements in the root mean square error (RMSE) across all state variables, with precipitation biases over land reduced by 25-35%, depending on the season. Beyond reducing climate biases, our approach enhances the representation of major modes of variability, including the North Atlantic Oscillation (NAO) and other key aspects of boreal winter variability. A particularly notable improvement is observed in the Madden-Julian Oscillation (MJO), where the CNN-corrected model successfully propagates the MJO across the maritime continent, a challenge for many current climate models. Using trio-interaction theory, we explore the dynamic improvements to the MJO and assess whether these enhancements arise from accurate physical processes.

 

This advancement underscores the potential of using CNNs for real-time model correction, providing a robust framework for improving climate simulations. Our findings highlight the efficacy of integrating machine learning techniques with traditional dynamical models to enhance climate prediction accuracy and reliability. This hybrid approach offers a promising direction for future research and operational climate forecasting, bridging the gap between observed and simulated climate dynamics.

How to cite: Chapman, W. and Berner, J.: Improving climate bias and variability via CNN-based state-dependent model-error corrections, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20624, https://doi.org/10.5194/egusphere-egu25-20624, 2025.

EGU25-3037 | Posters on site | CL3.2.3

METEOR - a spatially resolved impacts emulator 

Marit Sandstad, Benjamin Sanderson, and Norman Steinert

Introducing METEOR (Multivariate Emulation of Time-Evolving and Overlapping Responses) - a spatially resolved impacts emulator. P. Spatially resolved emulators can produce such data with a fraction of the computational cost required by full Earth system models, allowing the exploration of a much richer scenario space.

METEOR uses Earth system model output to emulate impact response patterns of varying decay timescales to forcing changes. As such, METEOR allows for the projection of future climate changes, including modelling of hysteresis in overshoot scenarios. In-built emissions to forcing mapping enables a full chain emulation of impact variables from emissions scenarios to spatially resolved impacts. METEOR can emulate multiple independent forcer responses, relying on at least one abrupt-CO2-change experiment as training data, and using either more abrupt forcer change experiments or a residual technique to emulate additional responses. This presentation will describe the model and its design philosophy and show results for emulations of CMIP6 model yearly mean temperature and precipitation. The flexibility of the framework allows application to a wide range of other more impact specific variables, and in addition the emulation patterns and timescales in themselves may reveal interesting patterns in the emulated data.

How to cite: Sandstad, M., Sanderson, B., and Steinert, N.: METEOR - a spatially resolved impacts emulator, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3037, https://doi.org/10.5194/egusphere-egu25-3037, 2025.

EGU25-5674 | Posters on site | CL3.2.3

A stochastic simulation strategy designed to study the future of extreme low flows in the context of electricity generation 

Sylvie Parey, Alexandre Devers, and Joël Gailhard

In a work published in 2022 (Parey and Gailhard 2022, [1]) a methodology designed to estimate extreme low flow, and based on stochastic modeling has been described and tested. This methodology was suited for a single watershed and involved a single site multivariate stochastic generator of consistent temperature and rainfall timeseries. Since then, methodological issues were raised, linked on the one hand to the hydrological modeling in a cascading basins context and on the other hand to the need of being able to produce and handle an ensemble of climate projections in a reasonable computing time. The first point refers to spatial added to multivariate consistency needed in the sub-basins to obtain coherent streamflow simulations, the second to the computational efficiency of the stochastic weather generator fitting and use.

Further investigations have shown that the multivariate stochastic generation was detrimental for the performance of the extreme events reproduction, especially for long heat waves such as the 2003 event in France. Furthermore, adding spatial consistency, in addition to the multivariate one, in the generator was not straightforward. Therefore, another weather generation strategy has been proposed and tested. It consists in using single variable generators, simple for precipitation and more sophisticated in the case of temperature for the purpose of heat wave projection, used independently and synchronized a posteriori through an empirical copula coupling approach linked with bootstrapping.

After a detailed description of the proposed approach to generate a large number of spatially and mutually consistent temperature and rainfall timeseries, its application to project future low flows in a French watershed of interest for electricity generation will be demonstrated with an example.

 

 

Reference:

[1] Parey, S.; Gailhard, J.: Extreme Low Flow Estimation under Climate Change. Atmosphere 2022, 13, 164. https://doi.org/10.3390/atmos13020164

How to cite: Parey, S., Devers, A., and Gailhard, J.: A stochastic simulation strategy designed to study the future of extreme low flows in the context of electricity generation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5674, https://doi.org/10.5194/egusphere-egu25-5674, 2025.

EGU25-6287 | ECS | Posters on site | CL3.2.3 | Highlight

AeroGP: machine learning how aerosols impact regional climate 

Maura Dewey, Annica Ekman, Duncan Watson-Parris, Anna Lewinschal, Bjørn Samset, Laura Wilcox, Maria Sand, Øyvind Seland, Srinath Krishnan, and Hans-Christen Hansson

Anthropogenic aerosol emissions have historically exerted a net cooling effect which has masked some of the simultaneous warming from greenhouse gases (roughly -0.5°C since pre-industrial times). This mean effect is the result of heterogenous climate forcing through aerosol-radiation and aerosol-cloud interactions both locally close to emission sources and remotely via teleconnections. Future reductions and shifts in aerosol emission patterns due to regional clean air policies and shifting industrial production could therefore unmask additional warming and induce spatially complex climate impacts. Therefore, there is a need for computationally efficient tools to assess the climate impacts of possible future aerosol policy decisions.

We have developed a machine-learning emulator using Gaussian Processes (GP), trained on output from the Norwegian Earth System Model (NorESM), to predict the global spatially resolved surface temperature response to regional aerosol emission perturbations. We use a novel design for our GP model which considers the joint spatial covariance of the outputs. We show the efficacy of the emulator is comparable to that of the parent model NorESM for a fraction of the computational cost, and then use it to assess potential future aerosol emission scenarios that might be relevant to European policy decisions.

How to cite: Dewey, M., Ekman, A., Watson-Parris, D., Lewinschal, A., Samset, B., Wilcox, L., Sand, M., Seland, Ø., Krishnan, S., and Hansson, H.-C.: AeroGP: machine learning how aerosols impact regional climate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6287, https://doi.org/10.5194/egusphere-egu25-6287, 2025.

EGU25-6759 | ECS | Posters on site | CL3.2.3

Statistical Emulation of Climate Impacts on Tourism Dynamics in Italy: Long-term Projections and Policy Implications  

Nguyen Thanh Thanh Duong, Flavio Pons, Ida D’Attoma, and Andrea Guizzardi

Understanding the long-term impacts of climate change on socio-economic systems requires computationally efficient methods that integrate complex climatological and economic processes. In this study, we employ statistical emulation techniques to project the impacts of climate change on domestic tourism demand in Italy through the year 2100. Using outputs from 22 regional climate models (RCMs) produced by the Coordinated Regional Climate Downscaling Experiment over Europe (EURO-CORDEX) project under RCP 4.5 and RCP 8.5 scenarios, we develop a statistical model that combines economic indicators (e.g., GDP and exchange rates) with climate variables such as temperature, solar radiation, and precipitation.

Non-linear effects of climate on tourism demand are also incorporated. By utilising statistical emulators, we achieve computational efficiency, enabling scenario analyses across diverse emissions pathways.

This research advances impact modelling for the tourism sector, illustrating how parsimonious statistical models can bridge the gap between complex Earth system simulations and practical applications in policy and industry. By quantifying these effects based on empirical evidence and widely accepted climate change projections, this study aims to inform mitigation policies and strategies that enhance sustainability and resilience in tourism destinations facing climate challenges. Ultimately, the findings are intended to influence policymakers and entrepreneurs, emphasising the need to address the long-term impacts of climate change on tourism demand.

How to cite: Duong, N. T. T., Pons, F., D’Attoma, I., and Guizzardi, A.: Statistical Emulation of Climate Impacts on Tourism Dynamics in Italy: Long-term Projections and Policy Implications , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6759, https://doi.org/10.5194/egusphere-egu25-6759, 2025.

EGU25-7013 | ECS | Posters on site | CL3.2.3

RIME-X: Emulating regional climate impact distributions using simple climate models and impact models 

Niklas Schwind, Mahé Perrette, Quentin Lejeune, Peter Pfleiderer, Annika Högner, Michaela Werning, Edward Byers, Anne Zimmer, Zebedee Nicholls, and Carl-Friedrich Schleussner

Simple climate models (SCMs) are widely used to simulate global mean temperature (GMT) trajectories across a wide range of emission scenarios by combining simplified representations of the carbon cycle and other Earth system processes. These simulations depend on uncertain Earth system parameters, and ensembles of SCM simulations are created by exploring plausible parameter sets, resulting in scenario-specific distributions of GMT for all considered years.

In this work, we introduce RIME-X (Rapid Impact Model Emulator Extended), a novel emulator approach that extends SCM outputs by translating GMT distributions into distributions of regionally aggregated climate or climate impact indicators. RIME-X uses historical and scenario simulations from climate and impact modeling intercomparison projects, such as CMIP and ISIMIP, to record relationships between global warming levels and indicators. By extracting distributions of indicators at specific global warming levels from those records and combining them with the GMT distributions from SCM ensembles, RIME-X produces scenario-dependent distributions of these indicators over time.

This framework integrates multiple sources of uncertainty along the modeling chain, including model uncertainty (from diverse climate or impact model records), Earth system parameter uncertainty (from SCM ensembles), and internal variability, depending on the indicator’s temporal resolution.

RIME-X is broadly applicable to any indicator whose distribution is predominantly influenced by the global warming level, offering a versatile and efficient tool for assessing climate impacts across a variety of scenarios. We demonstrate the capabilities of RIME-X by emulating a diverse set of regionally aggregated climate and climate impact variables available from ISIMIP3 and beyond for the NGFS (Network for Greening the Financial System) climate scenarios.

How to cite: Schwind, N., Perrette, M., Lejeune, Q., Pfleiderer, P., Högner, A., Werning, M., Byers, E., Zimmer, A., Nicholls, Z., and Schleussner, C.-F.: RIME-X: Emulating regional climate impact distributions using simple climate models and impact models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7013, https://doi.org/10.5194/egusphere-egu25-7013, 2025.

EGU25-9384 | ECS | Posters on site | CL3.2.3

Implementing global climate damage functions in a new Integrated Assessment Model 

Christopher Wells, Christopher Smith, Benjamin Blanz, Lennart Ramme, Ben Callegari, Muralidhar Adakudlu, Jefferson Rajah, Axel Eriksson, and Billy Schoenberg

The coupled interactions between components of the human-Earth system – impacts of human activity on the climate, and vice versa via climate impacts – are thought to be crucial determinants of the evolution of this system. However, the representation of these feedback loops is often minimal, or intentionally excluded, in existing integrated assessment modelling approaches.

The new global Integrated Assessment Model FRIDA v2.0 seeks to represent climate impacts as comprehensively as possible, at the global scale, focusing on high-level feedbacks between components of this system. This broad scope and high level of aggregation necessitates a reduced focus on individual impact channel complexity, with impacts simulated as functions of key global climate variables – e.g. temperature, CO2 concentration, and sea level rise.

Through this process, we have implemented key impact channels in FRIDA – on e.g. crops, energy supply and demand, mortality, and human behaviour. These channels generate substantial, complex effects on the evolution of the fully coupled human-Earth system.

In this presentation, we detail the process of collating and modelling climate impact channels within FRIDA v2.0, and present initial results of their overall effects on the system. We discuss the challenges of extracting internally consistent estimates from the literature, dealing with uncertainty across and between studies, conceptualising extremes. Finally, we discuss the need for future work to construct more comprehensive, consistent damage functions, and to coordinate their implementation in IAMs.

How to cite: Wells, C., Smith, C., Blanz, B., Ramme, L., Callegari, B., Adakudlu, M., Rajah, J., Eriksson, A., and Schoenberg, B.: Implementing global climate damage functions in a new Integrated Assessment Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9384, https://doi.org/10.5194/egusphere-egu25-9384, 2025.

EGU25-10007 | Posters on site | CL3.2.3

Build your own! From tailored box-model climate emulators to pattern scaling 

Doris Folini, Aryan Eftekhari, Aleksandra Friedl, Felix Kübler, Simon Scheidegger, and Olaf Schenk

Efficient and interpretable carbon-cycle emulators (CCEs) as part of climate emulators play a key role in Integrated Assessment Models. We present a framework enabling economists to custom-build purpose-tailored multi-reservoir linear box-model CCEs, accurately calibrated to advanced climate science. Three CCEs are presented for illustration: the 3SR model (replicating DICE-2016), the 4PR model (explicitly accounting for a land biosphere carbon reservoir), and the 4PR-X model, which accounts for dynamic land-use changes like deforestation that impact the reservoir's storage capacity and result in a time dependent CCE. We demonstrate that all three models are in line with benchmark data from comprehensive Earth System Models and exemplify how the dynamic land biosphere in the 4PR-X model impacts atmospheric carbon and temperature. The findings highlight the potential and relevance of use-cased tailored, efficient and interpretable climate emulators for economic studies. We complement our 'build your own CCE' toolbox by another set of statistical tools, commonly known as pattern scaling, that allows to go from the global mean temperature change obtained from the climate emulator to regional temperatures and changes thereof. The regional temperatures may be further translated into regional damages. We discuss the relative importance and uncertainty of each building block of this interpretable climate emulator chain, from (dynamic) CCE, to climate emulator, to pattern scaling.

How to cite: Folini, D., Eftekhari, A., Friedl, A., Kübler, F., Scheidegger, S., and Schenk, O.: Build your own! From tailored box-model climate emulators to pattern scaling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10007, https://doi.org/10.5194/egusphere-egu25-10007, 2025.

EGU25-11014 | Posters on site | CL3.2.3

Progress developing the PRIME framework and using it in FASTMIP.  

Camilla Mathison, Eleanor Burke, Gregory Munday, Chris Smith, Chris Jones, Chris Huntingford, Andy Wiltshire, Eszter Kovacs, Norman Steinert, Rebecca Varney, Laila Gohar, Michael Windisch, Yann Quilcaille, Sonia Seneviratne, and Daniel Hooke

Regionalized climate risk assessments are crucial for understanding impacts on ecosystems and society, and to allow planning for climate change. While existing Earth System Models (ESMs) provide a framework for such assessments, they often lack the critical processes simulated by dedicated Impact Models. However, Impact Models are often driven by output data from ESMs, which may need bias-correcting, and therefore, there is a significant time lag in the modelling chain. Furthermore, reliance on existing ESM data for Impact Models limits our analysis to the handful of scenarios (i.e. SSPs) and models that ran them (an “ensemble of opportunity” bias), while there is a need for multiple model simulations to try to capture uncertainty in future climate.


Over the last few years, we have developed the PRIME framework for producing scenarios of regional impacts for user-prescribed future emissions scenarios. PRIME combines global mean temperature and CO2 concentrations from the emissions driven FaIR simple climate model, as used in the IPCC Sixth Assessment Report, with patterns of climate change from CMIP6 (Coupled Model Intercomparison Project Phase 6) Earth System models to drive the JULES land surface model. This modelling framework projects regional changes to the land surface and carbon cycle. We will describe PRIME for the benefit of a new audience and demonstrate how this powerful and flexible approach answers questions on regional impacts using a range of scenarios. We will also talk about the FASTMIP modelling activity led by ETH Zurich with strong contributions of the UK metoffice and PNNL, which aims to provide a coordinated experiment of regional emulators for a wide range of scenarios. We will discuss how these systems tend to be flexible and fast to run and therefore represent a wealth of future development opportunities. In particular we will focus on how PRIME and similar frameworks will enable rapid probabilistic assessment of novel scenarios emissions scenarios that have not yet been run in ESMs thereby providing a useful insight and the capability to quantify societally-relevant climate impacts.

How to cite: Mathison, C., Burke, E., Munday, G., Smith, C., Jones, C., Huntingford, C., Wiltshire, A., Kovacs, E., Steinert, N., Varney, R., Gohar, L., Windisch, M., Quilcaille, Y., Seneviratne, S., and Hooke, D.: Progress developing the PRIME framework and using it in FASTMIP. , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11014, https://doi.org/10.5194/egusphere-egu25-11014, 2025.

EGU25-11101 | Posters on site | CL3.2.3

Evolution of the PRIME emissions-to-impacts modelling framework. 

Daniel Hooke, Camilla Mathison, David Sexton, Eleanor Burke, Andy Wiltshire, Chris Jones, and Laila Gohar

The PRIME emissions-to-impacts framework (Mathison et al. 2025) uses a chain of models, including the FaIR simple climate model and the JULEs land surface model, to simulate spatial resolved climate impacts and carbon cycle processes for policy relevant emissions scenarios. We present multiple updates to this framework, including a new methodology to sample large ensembles of the FaIR simple climate model, using an algorithm which maximises diversity across multiple dimensions (Sexton et al. 2021). The results are a sample with a more thorough representation of both atmospheric CO2 concentration and Global Mean Temperature. We use this sample to simulate the response of the carbon cycle under a more representative range of CO2 and temperature outcomes. In the latest version of PRIME we also include a more sophisticated representation of internal variability, and an updated daily climatology. A third methodological update is use of the PRIME framework with updated versions of JULES which include additional physical processes, such as permafrost physics and explicit representation of fire. This enables evaluation of processes not yet included in coupled Earth System Models. We use the PRIME framework in this configuration to model policy relevant overshoot scenarios, which gives us the opportunity to evaluate climate tipping points over a wide range of uncertainty. Finally, flexibility of the PRIME framework also allows us to provide driving data for other land surface models.

How to cite: Hooke, D., Mathison, C., Sexton, D., Burke, E., Wiltshire, A., Jones, C., and Gohar, L.: Evolution of the PRIME emissions-to-impacts modelling framework., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11101, https://doi.org/10.5194/egusphere-egu25-11101, 2025.

EGU25-11574 | Posters on site | CL3.2.3

Northern high latitude ecosystem carbon balance under climate change 

Eleanor Burke, Rebecca Varney, Daniel Hooke, Norman Steinert, Luke Smallman, Chris Jones, Gregory Munday, and Camilla Mathison

Recent studies suggest that the northern terrestrial permafrost region was a weak CO2 sink during the period 2000-2020. Future model projections remain highly uncertain – will the region remain a sink or become a source of CO2? And, if it becomes a source, when? Here we use a novel probabilistic framework PRIME (Probabilistic Regional Impacts from Model patterns and Emissions) constrained with observations to quantify a range of plausible pathways. Included are uncertainties in the global temperature response to emissions which are combined with uncertainties in spatial climate response to the global temperature change. This information is used to provide driving data for a range of JULES (the Joint UK Land Environment Simulator) configurations all of which include a representation of permafrost carbon to investigate the ecosystem carbon balance in the northern high latitudes.

How to cite: Burke, E., Varney, R., Hooke, D., Steinert, N., Smallman, L., Jones, C., Munday, G., and Mathison, C.: Northern high latitude ecosystem carbon balance under climate change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11574, https://doi.org/10.5194/egusphere-egu25-11574, 2025.

EGU25-13058 | ECS | Posters on site | CL3.2.3

Quantifying the Disproportionate Contributions of High-Income Groups to the Emergence of Climate Extremes 

Sarah Schöngart, Zebedee Nicholls, Roman Hoffmann, Setu Pelz, and Carl-Friedrich Schleussner

Climate change impacts are unevenly distributed, with those least responsible often bearing the brunt of its effects. This study quantifies how greenhouse gas emissions from high-income groups have influenced present-day global mean temperature levels and the frequency of temperature and potential drought extremes worldwide. We deploy an emulator-based modeling framework to systematically attribute changes in regional climate extremes to emissions from different wealth groups. 

Our results show that the wealthiest 10% globally contributed about 6.5 times the global average to warming (0.40°C ± 0.16°C), while the top 1% contributed 20 times the average (0.12°C ± 0.05°C). These disproportionate contributions are further amplified for extreme events, with the top 10% contributing about 7 times more to the emergence of 1-in-100 year heat and potential drought events than the global average. Emissions from the wealthiest 10% in the United States and China are associated with a two- to three-fold increase in the frequency of heat and drought extremes across vulnerable regions. This research provides a quantitative basis for discussions on climate equity and justice by linking wealth disparities to concrete climate change impacts. Our findings have important implications for designing effective and equitable climate policies that address both mitigation and adaptation needs. The study's application of a coupled MAGICC-MESMER-M-TP framework illustrates how emulator approaches can inform policy debates on differential responsibilities and capabilities in climate action, potentially supporting more targeted and just approaches to emissions reduction and climate finance.

How to cite: Schöngart, S., Nicholls, Z., Hoffmann, R., Pelz, S., and Schleussner, C.-F.: Quantifying the Disproportionate Contributions of High-Income Groups to the Emergence of Climate Extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13058, https://doi.org/10.5194/egusphere-egu25-13058, 2025.

EGU25-14775 | ECS | Posters on site | CL3.2.3

Advancing ProFSea: a spatially-resolved sea-level change emulator for long-term impacts  

Gregory Munday, Matthew Palmer, Rachel Perks, Lesley Allison, Jennifer Weeks, Chris Smith, and Jonathan Gregory

Sea-level rise simulation has previously been limited to Earth system models and global emulators - restricting spatially-resolved sea-level projections to those based on ageing emissions pathways with inflexible and expensive frameworks for updating projections using the latest scenarios. The ProFSea (Projecting Future Sea-level) tool improved on AR5 methods for fast regional sea-level prediction, but was limited to RCP scenarios and a 21st century timescale. We use the FaIR simple climate model to generate an ensemble of global surface temperatures from a range of policy-relevant scenarios, and drive a global sea-level rise simulator. The global projections are then localised using spatial patterns (derived from model estimates and observational evidence) related to key sea-level change drivers. Uncertainty is quantified and propagated throughout the modelling chain. We present the evaluation of this enhanced version of the ProFSea sea-level projections tool, and demonstrate its utility as a policy tool for predicting local sea-level change risk through the 21st century, out to 2300.

How to cite: Munday, G., Palmer, M., Perks, R., Allison, L., Weeks, J., Smith, C., and Gregory, J.: Advancing ProFSea: a spatially-resolved sea-level change emulator for long-term impacts , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14775, https://doi.org/10.5194/egusphere-egu25-14775, 2025.

EGU25-16962 | ECS | Posters on site | CL3.2.3

Statistical Emulations of Extreme Precipitation for Future Climate Scenarios 

Lorenzo Pierini, Lukas Gudmundsson, and Sonia Seneviratne

Extreme precipitation events have recently shown the potential to cause catastrophic flooding and damages, and the increasing effects of climate change are expected to intensify the associated socioeconomic and environmental risks. To facilitate the assessment of future scenarios, we extend the capabilities of the probabilistic emulator MESMER-X to represent extreme precipitation.
MESMER-X, designed to generate spatially resolved realizations of impact-relevant variables — such as annual maximum temperatures, fire weather, and soil moisture — for given global mean temperature trajectories, is adapted to emulate annual maximum daily precipitation.  Using data from CMIP6 Earth System Models across various Shared Socioeconomic Pathways, the emulator captures the underlying statistical distributions and spatial patterns, enabling the exploration of customized future scenarios at a fraction of the computational cost of fully coupled Earth System Models.  The performance of the emulation process is evaluated through probabilistic skill scores, residual analysis, and quantile comparisons with the original datasets.
MESMER-X outputs can support climate risk models in assessing future damages under policy-relevant scenarios, including those not previously explored with Earth System Models. This extension highlights the flexibility of MESMER-X in emulating a wide range of variables and provides a valuable support for analyzing precipitation-related climate impacts and potential targeted adaptation strategies.

How to cite: Pierini, L., Gudmundsson, L., and Seneviratne, S.: Statistical Emulations of Extreme Precipitation for Future Climate Scenarios, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16962, https://doi.org/10.5194/egusphere-egu25-16962, 2025.

Horizontal sampling of the ocean has been sparse for decades because of technical limitations. This can contribute to an incomplete depiction and misleading understanding of the hydrography. This is a particular concern for complex submesoscale and smaller scale flow structures that influence stratification and vertical transport of properties.

We use high resolution observations from a Triaxus towed undulating vehicle and develop a statistical subsampling pipeline in order to present the first multi-scale investigation of subsurface and interior horizontal density variability in a global context. Hydrographic transects were performed between 2018 and 2022 with vertical ranges extending from near-surface values down to depths varying between 50 and 350m in the oceanographically distinct regimes of the Arctic marginal ice zone, of a coastal upwelling area, of the equatorial Atlantic, and of the Antarctic Circumpolar Current. The investigation of lateral density gradient fields follows a baseline spanning four orders of magnitude, from 2m to 25km. Our main objectives are to determine the scaling properties of density fronts and to identify oceanic regimes that are susceptible to an underestimation of their thermohaline variability.

We find that the amplitude of horizontal density gradients increases non-linearly as the horizontal resolution is increased, closely following a proposed power law over all observed scales. This relation is applicable throughout all study regions allowing for a potential prediction of the gradient distribution for scales not resolved by measurements. Submesoscale density gradients are of higher amplitude along the base of shallow mixed layers, and in the presence of subsurface currents, frontal systems, and eddies. The latter two create strong lateral anisotropies in the density field, masking other contributions to the multi-scale spread of gradients. Furthermore, the gradient fields are primarily driven by salinity variability at high northern latitudes and by temperature variability in regions closer to the equator; in the Southern Ocean temperature and salinity largely compensate. The decay rate of the estimated gradients with increasing horizontal distance is related to fractal properties and a scale-dependent compensation of the density field.

This highlights that there is a certain arbitrariness regarding the strengths of density gradients in the present literature. We recommend that the employed horizontal resolution always be quoted alongside values of the horizontal density gradient.

How to cite: Duong, B. L. and von Appen, W.-J.: Scale Dependence of Subsurface Horizontal Density Gradients as Observed In-Situ Across Four Orders of Magnitude, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1518, https://doi.org/10.5194/egusphere-egu25-1518, 2025.

We analyze the tidal forcing effects on the internal variability in two marginal seas, the Bohai and Yellow Seas, and interpretate such effects from stochastic climate model and physical process (for instance, baroclinic instability) aspects. Ensemble simulations of the numerical module (Finite-volume Coastal Ocean Model) with and without tidal forcings are used to analyze the tidal forcing effects on the internal variability. EOF analysis is used to separate the variability into different spatial scales. The results show that the internal variability is significantly decreased especially in large (100 Km) and medium (60 km) scales, less so in small scales (23 km), when the tidal forcing is turned off. This result is well explained by Hasselmann's theory. Ocean memory, represented by the temporal autocorrelation function, is a critical element in this theory. Ocean memory is enhanced when the tidal forcing is excluded in all spatial scales, more obvious in large and medium scales; correspondingly, the internal variability increased significantly in the large and medium scales, compared with small scales in no-tide simulation. Physically, it can be explained as when the tidal forcing is turned off, once an anomaly appears in the system, it can survive for a longer time and easier to grow into large-scale variability. From the physical process aspect, we demonstrated that internal variability level and baroclinic instability variation co-vary consistently when comparing summer and winter seasons, and with and without tides. Our interpretation is that a stronger baroclinic instability causes more potential energy to be transformed into kinetic energy, allowing the unforced disturbances to grow.

How to cite: Lin, L. and von Storch, H.: The variability caused by external forcing and internal forcing in the marginal sea, Bohai and Yellow Sea , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4907, https://doi.org/10.5194/egusphere-egu25-4907, 2025.

EGU25-6284 | Posters on site | OS1.12

Estimation of the time-varying probability density function from ensemble simulations and observations using Analogs 

Benoît Presse, Sally Close, Pierre Tandeo, and Guillaume Maze

Understanding the role of ocean-atmosphere interactions is crucial in determining the drivers of ocean variability. Indeed, a part of this variability is not driven by the atmosphere but spontaneously and randomly generated by the ocean through non-linear processes. This internal variability is associated with multiple spatial and temporal scales, and may complicate the detection and attribution of climate change signals. Hence, quantifying the relative importance of atmospherically-forced and chaotic intrinsic variability is necessary to understand the mechanisms of climate change in the ocean-atmosphere system. However, both atmospherically-forced and intrinsic variability cannot be estimated with a single model experiment alone : an ensemble simulation approach is required. The ensemble mean approximates the component of the oceanic variability that is due to the influence of the atmosphere, while the spread represents the range of the estimated intrinsic variability. This work investigates the possibility of describing and predicting the random part of the ocean's variability from observations using an ensemble of ocean simulations in the North Atlantic ocean. An analog-based method is developed, and applied to Sea Surface Height data, with the aim of obtaining a less-computationally expensive method of estimating the time-varying probability function (PDF) that is normally obtained through ensemble simulation. The ensemble is supplied by the multi-decadal (1960-2015) global ocean/sea-ice eddy-permitting (1/4° resolution) large (50-member) ensemble simulation (OCCIPUT Experiment). The ensemble of SSH data as a whole provides the target PDF that we seek to estimate in a regions representative of the diversity of flows in the North Atlantic (e.g. at the centre of the North Atlantic gyre and in the Gulfstream current). The individual members are used to form the catalog of simulations in order to find analogs situations on which the estimate of the target PDF is based at time t. First results are promising and show that we are able to estimate the ensemble mean, but the variance is still a subject of active work due to the complexity of the shape of the PDF. The method greatly reduces the time and resources of computation by producing mean and variance of time-varying PDF for the entire time series in generally a few tens of minutes.

keywords : Internal variability, detection and attribution, model uncertainty, ocean-atmosphere interaction, predictability

How to cite: Presse, B., Close, S., Tandeo, P., and Maze, G.: Estimation of the time-varying probability density function from ensemble simulations and observations using Analogs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6284, https://doi.org/10.5194/egusphere-egu25-6284, 2025.

EGU25-6633 | ECS | Posters on site | OS1.12

Three-dimensional characteristic and variability of the current system in the western Pacific 

Jie-Hong Han and Jianping Gan

The ocean circulation system in the Western Pacific consists of western boundary currents (WBCs, Kuroshio Current, Mindanao Current, Ryuku Current) and connected with North Equatorial Current (NEC). The system is one of the most complicated current systems, vitally regulating the exchange of mass, energy, and heat transport between the open ocean and the adjacent marginal seas. Previous studies in Western Pacific circulations most focused on the variability of the circulations in specific sections without addressing the intrinsic connectivity and dynamics of currents in the system. Using the high-resolution, validated three-dimensional and time-dependent China Sea Multi-scale Ocean Modeling System (CMOMS, https://odmp.hkust.edu.hk/cmoms/), we quantitatively characterize the variability of the western boundary currents and related circulations in Western Pacific, and investigate their underlying physical processes. Based on physically sensible definitions of the jet stream and currents in the system, we identified characteristic width, depth, and along-/cross-stream transports and their unique spatiotemporal variability in the 3D current system. The momentum and vorticity analyses show the couplings between extrinsic inflow and intrinsic dynamic response of the Kuroshio Current in connections among currents in the system and between the marginal seas and open oceans. Synchronized structures in downstream variations of core velocity, cross-stream transport, eddy kinetic energy and path variability is pronounced along the Kuroshio Current. We found that the spatial patterns of Kuroshio are fundamentally modulated by mean flow-topography interactions, where shelf slope and shelf-current separation distance regulate the horizontal scales of the western boundary current, and thereby modify strain and shear characteristics and subsequent along-stream variability. The effect of topography on the synchronized spatial patterns is studied by energy budgets along the Kuroshio Current. Upstream influx and local flow-topography interaction acts as an external and internal forcing process to modulate the barotropic and baroclinic instability in Kuroshio variability, respectively. Associated time-averaged eddy fluxes are fundamentally reshape the mean current. By resolving three-dimensional, spatiotemporal variability of western current system, the study provides a new understanding to the dynamic connections in the Western Pacific Current system.

How to cite: Han, J.-H. and Gan, J.: Three-dimensional characteristic and variability of the current system in the western Pacific, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6633, https://doi.org/10.5194/egusphere-egu25-6633, 2025.

EGU25-7149 | Orals | OS1.12

Principle of equilibrium fluctuations 

Jin-Song von Storch

The ocean is forced by the fluxes of momentum, heat, and fresh water at the sea surface. When driving an ocean model using stationary fluxes for a sufficiently long time, we expect the model  to produce an equilibrated ocean characterized by stationary fluctuations. These fluctuations are not all synchronized with the surface fluxes.  For an ensemble obtained by forcing the ocean model with the same fluxes (starting from slightly different initial states),   fluctuations (at a time) that are  synchronized with the surface fluxes can be identified as the mean across the ensemble (at that time), and those not synchronized with the surface fluxes as the deviations from the mean across the ensemble. In case that the model has a sufficiently fine resolution, we expect that the latter — also known as intrinsic ocean variability — is substantial. The intrinsic ocean variability has to get its energy from somewhere. The only possible energy source is the surface fluxes, which originate from atmospheric motions supported (essentially) by the Sun. In this sense, intrinsic ocean variability can be considered as a feature of an ocean that is in equilibrium with a huge reservoir. 

 

The principle that governs equilibrium fluctuations — no matter how the equilibrium is reached — is a form of fluctuation-dissipation relation. The relation ensures that in an equilibrium with a reservoir, anything  that generates fluctuations must also dissipate fluctuations, and anything that dissipates fluctuations must also generate fluctuations. This principle makes a dynamical system in equilibrium with a reservoir be inherently random, even when the forcing resulting from the reservoir, such as the surface fluxes, is purely deterministic.  We evaluate this principle using solutions from the Lorenz's 1963 model and solutions obtained from the ICON ocean model with a horizontal resolution of  5 km. 

How to cite: von Storch, J.-S.: Principle of equilibrium fluctuations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7149, https://doi.org/10.5194/egusphere-egu25-7149, 2025.

EGU25-9954 | Posters on site | OS1.12

Modelling the phytoplankton community in a front: a Mediterranean Sea case study. 

Théo Garcia, Laurina Oms, Xavier Milhaud, Andrea Doglioli, Monique Messié, Claire Lacour, Pierre Vandekerkhove, Gérald Gregori, and Denys Pommeret

In the ocean, fine scales (1-100 km) are short-lived structures (days to weeks) that drive ocean physics, chemistry, ecology, and can influence climate. Among them, fronts are ubiquitous fine-scale physical features that separate different water masses and create gradients of biogeochemical contents. Fronts are often associated with vertical mixing of the water column, allowing the availability of nutrients that support phytoplankton dynamics. However, how such structures affect phytoplankton distribution is not well understood, especially in oligotrophic regions. We hypothesize that the phytoplankton community observed in the frontal zone is a mixture of communities observed in the adjacent water masses, plus another community.

Here, we are interested in the community composition based on nine phytoplankton functional types (PFTs) observed by flow cytometry in a front, in the western oligotrophic Mediterranean Sea. During the PROTEVSSWOT MED cruise (doi:10.17183/protevsmed_swot_2018_leg2), south of the Balearic Islands, high-resolution measurements allowed us to collect samples in the front and the two adjacent water masses along a strong salinity gradient.

Our objective is to model the frontal phytoplankton community as a finite mixture of the adjacent water mass communities A and B, and a new community C. In this model, we specified that the communities in the adjacent water masses and the new community can arise from a discrete mixture of multivariate normal distributions. First, we estimated the parameters and number of components in the finite mixture for the adjacent water mass communities A and B using an Expectation Maximization algorithm. From a larger dataset, we estimated the parameters of a set of likely communities for C. Then, we developed a hierarchical Bayesian model to estimate the weight of each component of the discrete mixture. Finally, the hierarchical Bayesian model was run a second time using only the most significant components for community C.

One component was sufficient to model community A (North to the front), while communities B (South to the front) and C were modeled with two components. The new community C explained a significant part of the frontal community. With very few observations in the frontal zone (n=11), our Bayesian approach highlighted the spatial distribution of the phytoplankton community around the front. Our result suggests that local environmental conditions in the front allow the emergence of a new community. This work is a first step in understanding frontal zones in an oligotrophic region, representative of the global ocean. Our modeling approach will be further applied in a larger dataset (BIOSWOT-MED cruise, doi:10.17600/18002392). In these further analyses, environmental data will be included to disentangle the physical-biological processes that shape phytoplankton distribution.

This work was funded by the Institut des Mathématiques pour la Planète Terre which supports collaborations between mathematicians and life and earth sciences.

How to cite: Garcia, T., Oms, L., Milhaud, X., Doglioli, A., Messié, M., Lacour, C., Vandekerkhove, P., Gregori, G., and Pommeret, D.: Modelling the phytoplankton community in a front: a Mediterranean Sea case study., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9954, https://doi.org/10.5194/egusphere-egu25-9954, 2025.

EGU25-10891 | ECS | Orals | OS1.12

Past, Present, and Future Variability of Atlantic Meridional Overturning Circulation in CMIP6 Ensembles 

Arthur Coquereau, Florian Sévellec, Thierry Huck, Joël Hirschi, and Quentin Jamet

The Atlantic Meridional Overturning Circulation (AMOC) is a key component of the climate system, exhibiting strong variability across daily to millennial timescales and significantly influencing global climate. Sensitive to external conditions such as freshwater input, greenhouse gas concentrations, and aerosol forcing, important variations of the AMOC can be triggered by anthropogenic emissions. This study presents a comprehensive analysis of sources of AMOC variance in state-of-the-art climate ensemble models. By decomposing the effects of scenario, model, ensemble, and time variability, along with their interactions, through an Analysis of Variance (ANOVA), we identify three distinct regimes of AMOC variability from 1850 to 2100. The first regime, spanning most of the historical period, is characterized by a relatively stable AMOC dominated by internal variability. The second regime, initiated by AMOC decline at the end of the 20th century and lasting until mid-21st century, is governed by a transient increase of time variability. Notably, the direct effect of forcing differences remains muted all along this regime, despite the start of emission-scenarios in 2015. The third regime, beginning around 2050, is marked by the emergence and rapid dominance of inter-scenario variability. Throughout the simulations, model variability remains the primary source of uncertainty, influenced by aerosol forcing response, AMOC decline magnitude, and the physical variability. A key finding of this work is the evidence that internal variability decreases simultaneously with AMOC intensity and seems proportional to emission-scenario intensity. 

How to cite: Coquereau, A., Sévellec, F., Huck, T., Hirschi, J., and Jamet, Q.: Past, Present, and Future Variability of Atlantic Meridional Overturning Circulation in CMIP6 Ensembles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10891, https://doi.org/10.5194/egusphere-egu25-10891, 2025.

EGU25-12552 | ECS | Orals | OS1.12

Ensemble Ocean Simulations in the North Atlantic: Exploring the Intrinsic Variability in Subtropical Mode Water Dynamics 

Luolin Sun, William Dewar, Bruno Deremble, Nicolas Wienders, and Andrew Poje

The non-linear nature of the ocean dynamics motivates the use of ensemble ocean simulations to discriminate the intrinsic and extrinsic sources of oceanic variability. Separating the mean and eddy flows from ensemble statistics also gives access to their local and instantaneous interactions in the non-stationary and inhomogeneous ocean. We here take advantage of this idea to quantify the local/instantaneous roles of laminar and eddy fluxes in the seasonal cycle of the North Atlantic subtropical mode water (STMW) that is formed through ocean-atmosphere interaction and controls large-scale oceanic ventilation.

We employ an ensemble of 48 North Atlantic 1/12-degree ocean simulations, where all members are driven by the same atmospheric forcing after slight initial perturbations. We achieve a space/time-dependent mean-eddy flow separation by obtaining a residual-mean flow that represents the common oceanic response of all ensemble members to the atmosphere, and a set of residual eddies that reflect the ensemble dispersion. We characterise the STMW as a low Ertel potential vorticity (PV) pool and find that its PV budget is mostly controlled by the ensemble mean PV flux: the formation and erosion of the STMW is predominantly driven by the residual-mean flow. The contribution of eddy PV transport is secondary; this can be attributed to the low intrinsic variability within the PV pool, as captured by the residual eddies. 

Overall, our results show that ensemble ocean simulations are powerful to investigate inhomogeneous, non-stationary, nonlinear multiscale ocean dynamics, providing deeper insights into the life cycle of large-scale climate-relevant features like STMW.

How to cite: Sun, L., Dewar, W., Deremble, B., Wienders, N., and Poje, A.: Ensemble Ocean Simulations in the North Atlantic: Exploring the Intrinsic Variability in Subtropical Mode Water Dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12552, https://doi.org/10.5194/egusphere-egu25-12552, 2025.

EGU25-14639 | Orals | OS1.12

Intrinsic interannual variability of the Indonesian Throughflow 

Ryo Furue, Masami Nonaka, and Hideharu Sasaki

The Indonesian Throughflow (ITF) carries an annual average of about 15 Sv of water from the Pacific through the Indonesian Seas Into the Indian Ocean, and its year-to-year variation ranges from 1 to 4 Sv. A 10-member ensemble of 41-year integrations of a semi-global eddy-resolving oceanic general circulation model is examined to explore the intrinsic (chaotic) variability of the ITF transport and associated flow. It is found that the annual-mean ITF transport is different by about 1 Sv between the ensemble members at several years. The characteristic vertical and horizontal structures of the ensemble anomaly (deviation from the ensemble average) are described. These structures and the basin-scale spread of the anomaly suggest that the intrinsic variability of the ITF is a genuine increase or decrease of the classical ITF rather than variability due to local eddies or nonlinear currents within the Indonesian Seas. The lagged correlation of the intrinsic component of the ITF transport with sea-surface height and barotropic streamfunction suggests that the intrinsic variability may come from zonal jets in the western subtropical North Pacific.

How to cite: Furue, R., Nonaka, M., and Sasaki, H.: Intrinsic interannual variability of the Indonesian Throughflow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14639, https://doi.org/10.5194/egusphere-egu25-14639, 2025.

Ensemble ocean model experiments can be useful to understand the extent to which internal variability has exerted an influence on a given observation, or indeed modelled event. This is important in contexts such as that of ongoing climate change, for example, where this probabilistic information can be useful for the purposes of detection and attribution. However, ensemble simulation has certain disadvantages, including its very high computational and energetic cost, the technical skill required to implement such modelling strategies, and the inherent dependence of the results on model physics. The aim of this study is to address these drawbacks by directly estimating the ensemble mean using statistical methods applied to individual model simulations, or observations. The effects of internal variability should be strongly reduced in these artificial ensemble mean estimates, enabling better insight into the direct effects of atmospheric forcing on the chosen ocean variables.

In previous work, we showed that the ensemble mean sea surface height can be estimated with good accuracy by filtering an individual member of the ensemble. Here, we extend this result to sea surface temperature (SST), which requires a more complicated spatiotemporal filter to estimate the ensemble mean, but again shows good agreement with the true ensemble mean SST at very low computational cost. However, examination of the full 3D temperature fields show a more complicated spectral coherence signature, suggesting that application of the filtering method to these 3D fields would be more challenging. In a second step, a neural network is thus trained to reproduce 3D ocean temperature fields using SST and sea surface height as inputs. By combining the filtered fields with the neural network, first estimates are made of the ensemble mean 3D temperature field, based on observations. Comparisons with the true ensemble mean 3D fields are encouraging, and suggest that the method may be useful as a cheap alternative to numerical simulation to better identify the atmospheric influence on ocean variability.

How to cite: Close, S. and Penduff, T.: Estimates of artificial ensemble mean ocean properties from individual simulations and observations to better isolate the atmospheric influence on ocean variability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15192, https://doi.org/10.5194/egusphere-egu25-15192, 2025.

EGU25-15591 | ECS | Orals | OS1.12

A stochastic framework for modeling surface ocean variability in the Southwest Indian Ocean 

Lisa Weiss, Jean-Michel Brankart, Quentin Jamet, and Pierre Brasseur

The Southwest Indian Ocean (SWIO) is characterized by diverse dynamic regimes, with intense energy fluxes and intricate atmospheric interactions (Phillips et al., 2021, OS). The Mascarene area, to the east of Madagascar, is influenced by the South Equatorial Current and the Indian subtropical gyre, the Mozambique Channel presents numerous mesoscale eddies, which play an important role in the biogeochemical dynamics, and the Equatorial zone is affected by the inversion of seasonal Monsoon circulation. Modeling such complex systems requires the consideration of multiple sources of uncertainty. In the context of global warming and climate projections, it is essential to simulate these uncertainties in order to obtain a more accurate representation and understanding of the SWIO ocean dynamics. The objective of this project is to identify and analyze the dominant sources of uncertainty affecting surface circulation in the SWIO. To address this issue, a probabilistic approach is integrated into the CROCO model (Coastal and Regional Ocean Community), following three key steps. Firstly, a realistic regional configuration of the CROCO model is developed for the SWIO region, which is forced and validated by CMEMS and ECMWF operational and satellite products. Then, a stochastic perturbation generator (referred to as STOGEN and originally developed in the NEMO model, Brankart et al., 2015, GMD) is implemented into CROCO, associated with an ensemble generator. Finally, several ensemble simulations are performed using stochastic processes with varying correlation structures in space and time within the defined regional setting. This allows to test the cumulative effect of different sources of uncertainty associated with surface ocean circulation by analyzing the ensemble statistics and variability based on surface variables such as sea surface height, temperature, salinity or velocity fields. We starts with the simulation of an ensemble by perturbing the wind stress. Then, three additional ensemble simulations will be generated by perturbing the vertical mixing, the initial conditions to analyze the intrinsic ocean variability and the open boundary conditions. The integration of stochastic parameterization within CROCO allow to simulate and partially quantify some of the non-deterministic effects of unresolved processes and scales. It enables an objective statistical comparison between model and observations associated with uncertainty description for data assimilation systems (Popov et al., 2024, OS).

How to cite: Weiss, L., Brankart, J.-M., Jamet, Q., and Brasseur, P.: A stochastic framework for modeling surface ocean variability in the Southwest Indian Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15591, https://doi.org/10.5194/egusphere-egu25-15591, 2025.

EGU25-16511 | Posters on site | OS1.12

A multi-centennial ocean simulation reveals aspects of the Mediterranean Sea intrinsic dynamics 

Angelo Rubino, Michele Gnesotto, Davide Zanchettin, and Stefano Pierini

A multi-centennial ocean simulation focusing on the Mediterranean Sea intrinsic dynamics is performed using an eddy-permitting nonlinear, shallow-water multilayer numerical model forced by steady transports of Atlantic Water and Levantine Intermediate Water. These transports are prescribed along two western and eastern open boundaries located along meridional sections crossing the strait of Gibraltar and the Levantine basin, respectively. Low-frequency oscillations in the inflowing Atlantic Water density are imposed, which mimic the effect of long-term North Atlantic variability on the water masses entering the Mediterranean basin. In this contribution we compare the simulated annual mean surface displacements with corresponding absolute dynamic topography altimetric observations. This research is supported by the Italian INVMED-P.R.I.N. project.

How to cite: Rubino, A., Gnesotto, M., Zanchettin, D., and Pierini, S.: A multi-centennial ocean simulation reveals aspects of the Mediterranean Sea intrinsic dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16511, https://doi.org/10.5194/egusphere-egu25-16511, 2025.

EGU25-17449 | ECS | Orals | OS1.12

A Stochastic description of eddy-mean flow interactions 

Mattéo Nex, Quentin Jamet, Etienne Mémin, and Florian Sévellec

When studying large tuburlent regions of the ocean, interactions between the mean flow and eddies plays a
central role in shaping large-scale circulation patterns by redistributing heat, momentum, and energy across the
ocean. Accurately representing these interactions in General Circulation Models (GCMs) remains a challenge,
particularly due to the subgrid-scale modelling issues and the limitations of traditional parameterization methods.
In this study we highlights the limitations of the diagnostics that can be performed with a too small in size en-
semble of simulations for capturing the Reynolds stress tensor as well as accurately diagnosing the work of such
tensor. In the context of studying energy exchange between the mean flow and eddies, the work of the Reynolds
stress is associated with the mean-to-eddy energy conversion rate MEC (Jamet et al. 2022).

To address the above issues, we explore the capabilities of the Location Uncertainty (LU) framework (Mémin
2014) to provide a better representation of eddy-mean flow energy transfer. By introducing stochastic variability
directly into the governing equations of fluid motion, LU provides an approach to model the unresolved turbulent
effects. A rederivation of the equation for the energy transfers is then possible through a stochastic version of
the Reynolds Transport Theorem (Bauer et al. 2020) and leads to an alternative representation of the interactions
between mean flow and eddies.

Based on 48-member ensemble simulation of the North Atlantic under realistic forcing, we provide a robust
comparison between deterministic and stochastic estimates of the work of Reynolds stress (MEC). By comparing
deterministic and stochastic estimates of MEC, we show that LU can effectively address the issues of stastistical
convergence by inflating intrinsic variability leading to a more robust representation of these non-linear terms. In
addition, statistical moments are shown to be more stable than from the deterministic formulation of the eddy-mean
flow interactions. Key results of this study include a detailed formulation of kinetic energy evolution equations
under the LU framework, which reveals significant improvements compared to the deterministic formulation of
the work of the Reynolds stress in terms of statistical moments. The noise definition relies, in this study, on the
snapshot proper orthogonal decomposition (POD) in the ensemble dimension, offering a time varying orthogonal
eigenfunctions basis. These diagnostics provide usefull tools to observe moving patterns and stability regions,
leading to physical interpretation of the eddy-mean flow interactions in the Gulf Stream.

How to cite: Nex, M., Jamet, Q., Mémin, E., and Sévellec, F.: A Stochastic description of eddy-mean flow interactions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17449, https://doi.org/10.5194/egusphere-egu25-17449, 2025.

EGU25-19468 | Orals | OS1.12

Where, why, and over which timescales is coastal sea-level potentially predictable? 

Chris Wilson and Simon D. P. Williams

In some places and over some time horizons, coastal sea-level is highly predictable. For example, there are locations where the seasonal cycle dominates and the monthly-mean sea- level is predictable for many years ahead. However, in other places, we know that there are frequent storm surges, that AMOC changes are linked to coastal sea-level, that mass anomalies propagate around the continental shelf slope boundary and can affect remote changes in coastal sea level, but also that there is a manifestation of internal or intrinsic, nonlinear processes which have a chaotic signature. From place to place, globally, there is a need to optimally predict coastal sea-level for societal planning and adaptation, to mitigate the effects of climate change and sea-level rise. However, on the regional and local scales, there are still many gaps, both in terms of observation and modelling of coastal sea-level on timescales relevant to people’s lives and wellbeing.

 

Using an ensemble modelling approach, one can use the ensemble mean and ensemble variance to estimate a potentially predictable,”forced” component of the system and a potentially unpredictable, ”unforced” component. In terms of sea-level, the unforced, chaotic intrinsic variability (CIV) component can, in some locations, dominate the forced component, even out to decadal timescales. This is known to be a major source of uncertainty in sea-level trends, relevant to IPCC projections, but analogously so for other temporal components on seasonal to decadal timescales too.

 

This study:

  • a) verifies where and over which timescales of variability the OCCIPUT, eORCA025, 50- member initial condition ensemble simulation captures coastal sea-level from the GESLA3 tide gauge dataset.
  • b) generates maps of the potential predictability of coastal sea-level.
  • c) explores predictive suitability of statistical models versus GCMs.
  • d) suggests relevant processes behind potential predictability characteristics.

How to cite: Wilson, C. and Williams, S. D. P.: Where, why, and over which timescales is coastal sea-level potentially predictable?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19468, https://doi.org/10.5194/egusphere-egu25-19468, 2025.

EGU25-20796 | ECS | Orals | OS1.12

Forced and Intrinsic Low-Frequency Variability in the Mediterranean Sea from a Multi-Decadal Ensemble Simulation 

Damien Héron, Jean-Michel Brankart, and Pierre Brasseur

This study investigates the low-frequency variability of the Mediterranean Sea using an ensemble of 30 eddy-permitting (1/12°) NEMO-based regional ocean simulations. The ensemble members were slightly perturbed in their initial conditions and forced by the same atmospheric variability during 34 years, allowing us to separate the intrinsic and atmospherically-forced components of the ocean variability.

At interannual timescales, our analysis of sea surface height (SSH) reveals distinct patterns of intrinsic variability across the basin. While the variability of certain circulation features, such as the North Ionian Gyre (NIG), is mostly paced by the atmosphere, low-frequency fluctuations of other features —like in the Algerian Basin— are largely intrinsic and random. The variance decomposition reveals that intrinsic processes control most of the total SSH variability over one-fifth of the basin, highlighting their pivotal role in shaping the interannual fluctuations in the basin.

Inspired by previous studies of the Atlantic Meridional Overturning Circulation (Gregorio et al., 2015; Leroux et al., 2018), we investigate the forced and intrinsic components of the Mediterranean Zonal Overturning Circulation (ZOC) interannual variability, focusing on the eastward flow of Atlantic waters and westward flow of intermediate waters in density coordinates. While the transport in the western basin shows moderate variability, our results reveal an increase in total variability in the Levantine Basin, driven by both forced and intrinsic components. EOF analyses of ZOC fluctuations suggest distinct variability modes east and west of Sicily, which remain to be further investigated.

This work highlights the substantial contribution of intrinsic variability in various features of the Mediterranean's fluctuations, up to decadal timescales. A better understanding of the relative contributions of externally-driven and internally-generated oceanic fluctuations is crucial for accurately interpreting simulated and observed signals, making reliable predictions, and exploring possible impacts on marine ecosystems.

How to cite: Héron, D., Brankart, J.-M., and Brasseur, P.: Forced and Intrinsic Low-Frequency Variability in the Mediterranean Sea from a Multi-Decadal Ensemble Simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20796, https://doi.org/10.5194/egusphere-egu25-20796, 2025.

EGU25-530 | ECS | Orals | HS7.2

Improving Precipitation Merging: A Generalized Two-Stage Framework Using the Signal-to-Noise Ratio Optimization (SNR-opt) 

Seokhyeon Kim, Suraj Shah, Yi Liu, and Ashish Sharma

Gauge-independent, multi-source precipitation merging methods are well-established approach for improving precipitation estimates. These methods predominantly aim to minimise uncertainty in precipitation magnitude, yet they frequently neglect errors in distinguishing between rain and no-rain events. This oversight often leads to biased merging weights and suboptimal precipitation estimates. In this study, we introduce an innovative two-stage framework called the Generalised Signal-to-Noise Ratio Optimisation (G-SNR) framework, specifically designed to address these limitations. The first stage employs the Categorical Triple Collocation-Merging (CTC-M) method for binary merging, effectively mitigating errors in rain/no-rain classification. The second stage applies Signal-to-Noise Ratio Optimisation (SNR-opt) to enhance precipitation magnitude estimates, leveraging the improved classification outcomes. Evaluation results demonstrate that G-SNR consistently surpasses both input data and existing methods in terms of binary classification and magnitude estimation. Importantly, it achieves error reductions across all percentiles, delivering robust performance for both low and extreme precipitation events. This framework provides a comprehensive and reliable solution to longstanding challenges in precipitation merging, significantly enhancing both accuracy and dependability.

How to cite: Kim, S., Shah, S., Liu, Y., and Sharma, A.: Improving Precipitation Merging: A Generalized Two-Stage Framework Using the Signal-to-Noise Ratio Optimization (SNR-opt), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-530, https://doi.org/10.5194/egusphere-egu25-530, 2025.

Reliable precipitation data from in-situ stations is often limited by inconsistent quality, resolution, and spatial coverage. This is particularly true in regions like the West Bank, where ground-based observations are scarce. This hampers hydrological and environmental studies where accurate precipitation estimates are vital.  Therefore, satellite-based rainfall products are an appealing alternative due to their broad spatial and consistent temporal coverage. However, the accuracy of these products in complex terrain is questionable due to sensor and retrieval errors, necessitating adjustment to improve their reliability. This study evaluates various adjustment methods for four satellite precipitation products (IMERG Final Run, PDIR-Now, CCS-CDR, and CMORPH) across the study area of Historical Palestine (West Bank and Israel). Daily satellite precipitation estimates were compared to observations from 316 in-situ stations (256 in Israel and 58 in the Palestinian territories). Adjustment methods included traditional bias correction techniques (Linear Scaling, Daily Translation, and Annual Sums), more advanced approaches (Empirical Quantile Mapping, Robust Quantile Mapping, Gaussian Distribution Mapping, and Local Intensity Scaling), and machine learning models (Random Forest and Artificial Neural Networks). Results show that, among the non-machine learning approaches, Daily Translation (DT) achieved the greatest improvement in accuracy followed by Power Bias adjustment. DT applied to IMERG resulted in an improvement of 24% and 17% in R2 and Mean Absolute Error (MAE) respectively. All machine learning approaches outperformed non-machine learning methods, with a two-step Random Forest (RF2) method delivering the best results. RF2, which leverages data from multiple satellites, had a 109% improvement in R2 and a 54% improvement in MAE. Additionally, the global RFG model showcased excellent results in producing a unified model that can be generalized for the entirety of the study area. The findings are globally applicable and evaluate multiple adjustment methods which opens the opportunity for easily accessible remotely sensed precipitation products to be used in many hydrological applications.

How to cite: Jayousi, F. and O'Loughlin, F.: Precision in Precipitation:  Bias Corrections and Machine Learning for Reliable Satellite Precipitation in The Levant, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-722, https://doi.org/10.5194/egusphere-egu25-722, 2025.

EGU25-841 | ECS | Orals | HS7.2

Urban runoff response to climate-change-driven heavy precipitation and urbanization 

Raz Nussbaum, Moshe Armon, and Efrat Morin

Excess runoff from heavy precipitation events (HPEs) in urban environments often leads to urban flooding, a severe hazard with significant implications for human life, property, and infrastructure. Modeling runoff response in complex and heterogeneous urban areas, while accounting for rainstorm and surface characteristics, remains a significant challenge. Climate change and urbanization are key drivers of increased future urban runoff intensity. Research on the interaction between these factors and urban runoff in the eastern Mediterranean region is particularly limited. Previous studies using high-resolution models have projected an increase in short-duration rainfall intensities, alongside a decrease in long-duration intensities, rainfall coverage area, and total event rainfall during HPEs in the eastern Mediterranean under the RCP8.5 scenario. The current study examines the implications of these changes on peak discharge and volume of urban runoff by the end of the 21st century and evaluates the influence of varying urbanization scenarios, providing insights into the interplay between climate change and urban development. Using high-resolution radar-rainfall and surface data, we developed and calibrated a SWMM-based urban rainfall-runoff model for the Nahal Ra'anana basin (13 km²) on Israel's coastal plane. This Mediterranean-climate region encompasses most of the city of Ra'anana and has approximately 40% impervious surfaces. The model was developed using 23 runoff events utilizing leave-one-out cross-validation and a multi-objective optimization approach, and demonstrated robust performance with KGE values of 0.80 for runoff peak discharge and 0.83 for total runoff volume. A variance-based sensitivity analysis identified three primary factors influencing urban runoff: rainstorm intensity distribution, impervious surface coverage, and basin water storage. Analysis of HPEs under historical and future climatic conditions revealed that, at the current urbanization level of the city, climate change alone is unlikely to alter peak or total runoff discharge significantly. This is attributed to the decrease in total event rainfall and coverage area, alongside an increase in short-duration rainfall intensities. However, with substantial urbanization (e.g., increasing impervious surface to 52% or more), future climate HPEs are expected to exhibit a noticeable shift in the trend, leading to increased peak discharge. Further analysis indicates the elevated importance of rainfall intensities in determining runoff peaks in future climate conditions. In historical HPEs the maximum rainfall intensities over a 60-minute duration strongly correlate with peak runoff discharge (R2=0.75), where in future climate HPEs, correlations of shorter and longer rainfall durations are improved compared to historical HPEs with the maximum obtained for 60–120-minute durations (R2=0.81). The non-linear discharge response to climate change underscores the importance of integrating climate projections into urban planning to mitigate future flooding risks and highlight the potential for short-term peak discharge forecasting under both current and future climatic conditions.

 

How to cite: Nussbaum, R., Armon, M., and Morin, E.: Urban runoff response to climate-change-driven heavy precipitation and urbanization, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-841, https://doi.org/10.5194/egusphere-egu25-841, 2025.

EGU25-1018 | ECS | Posters on site | HS7.2

Statistical Downscaling Techniques and Projection of Future Climate Extremes in the Sudano Sahelian Environment 

Ibrahim Njouenwet and Jérémy Lavarenne

The Sudano-Sahelian Region of Cameroon (SSRC) faces significant challenges due to high rainfall variability and rapid population growth. Despite long-standing adaptation strategies, the region's vulnerability to climate variability and change remains a critical concern, prompting extensive research and calls for greater adaptation funding. In Sahelian West Africa, the decline in rainfall stations has significantly reduced data availability, hindering the calibration and evaluation of climate models and limiting their ability to accurately represent the region's climate. However, there are notable discrepancies between global and regional models regarding projected changes in precipitation patterns across specific regions and seasons, particularly in areas like the Eastern Sahel region, which includes the SSRC. Bias correction (BC) and downscaling (DS) are crucial, as these bias can be propagated into impact models. This study aims to fill the gap of localized and reliable information for climate services in the Sudano Sahelian region.

Using high-resolution rainfall data from NoCORA—daily interpolated rainfall maps for Northern Cameroon based on 418 stations (1948–2022) at 0.01° resolution (Jérémy et al., 2023)—the 25-km resolution regional climate models derived from a CMIP5 model are employed to better capture the climatology of extreme precipitation events, with kilometer-scale bias correction applied to outputs over the study area. Additionally, a subset of CMIP6 simulations is statistically downscaled to evaluate local-scale model uncertainties and compare the effectiveness of statistical and dynamical downscaling methods.

This study evaluates the performance of four state-of-the-art statistical downscaling techniques namely Linear Scaling, CDF-t, Quantile Mapping and Quantile DeltaMapping using different metrics and compares extreme precipitation changes under climate change scenarios to identify a suitable method for correcting bias in climate models projections for the period 2005-2100. The findings of this study will help impact modelers by enhancing the application of bias adjustment methods, thereby supporting the development of robust local climate change impact assessments in agriculture and hydrology domains.

Keywords : extreme precipitation, biais correction, Statistical downscaling, climate models

How to cite: Njouenwet, I. and Lavarenne, J.: Statistical Downscaling Techniques and Projection of Future Climate Extremes in the Sudano Sahelian Environment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1018, https://doi.org/10.5194/egusphere-egu25-1018, 2025.

EGU25-2058 | ECS | Posters on site | HS7.2

Refining Rainfall Erosivity Estimation: Methodological improvements towards more accurate soil erosion assessments 

Athanasios Serafeim, Roberto Deidda, Paolo Nasta, Nunzio Romano, Dario Pumo, and Andreas Langousis

Rainfall erosivity is a fundamental parameter in estimating soil erosion as it quantifies the potential of raindrops to detach soil particles and make them available for subsequent transport by surface runoff. Erosivity depends mainly on the intensity, duration, and energy of precipitation events, which directly affect the impact of raindrops on the soil surfaces and runoff. The most common methods for identifying erosive events emphasize short-duration, high-intensity rainfall events, while introducing critical thresholds for characterizing erosive events, such as the 30-minute maximum rainfall intensity (I30) and storm separation criteria (see e.g. Wischmeier and Smith, 1978, Foster et al., 1981 and Renard et al., 1997).

Nevertheless, both historical and recently proposed frameworks occasionally consolidate rainfall events that should be disaggregated according to the established six-hour dry period threshold, leading to overestimation of rainfall event durations and erosivity factors. The present study aims at refining the identification and analysis of erosive rainfall events, a key component of soil erosion prediction, by introducing an alternative approach that strictly adheres to the original criteria introduced by Wischmeier and Smith (1978) and Renard et al. (1997), ensuring precise segmentation of rainfall events when rainfall accumulation is below the 1.27 mm threshold over a six-hour period.

The proposed method classifies rainfall events as erosive when total rainfall exceeds 12.7 mm or meets intensity thresholds of 6.4 mm in 15 minutes or 12.7 mm in 30 minutes. Comparative analysis with existing approaches demonstrates improved alignment with fundamental criteria while addressing modern computational challenges, contributing to the advancement of soil erosion prediction by bridging historical methodologies with contemporary analytical precision.

References

Wischmeier, W.H., Smith, D. D. (1978) Predicting rainfall erosion losses: A guide to conservation planning. Agric. Handb. 537. US Gov. Print. Office, Washington, DC.

Foster, G.R., McCool, D.K., Renard, K.G., Moldenhauer, W.C. (1981) Conversion of the universal soil loss equation to SI metric units. J. Soil Water Conserv. 36, 355–359.

Renard, K., Foster, G., Weesies, G., McCool, D. and Yoder, D. (1997) Predicting Soil Erosion by Water: A Guide to Conservation Planning with the Revised Universal Soil Loss Equation (RUSLE). US Department of Agriculture, Agriculture Handbook No.703USDA, USDA, Washington DC.

How to cite: Serafeim, A., Deidda, R., Nasta, P., Romano, N., Pumo, D., and Langousis, A.: Refining Rainfall Erosivity Estimation: Methodological improvements towards more accurate soil erosion assessments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2058, https://doi.org/10.5194/egusphere-egu25-2058, 2025.

EGU25-2770 | Posters on site | HS7.2

A new tool for correcting the spatial and temporal pattern of global precipitation products across mountainous catchments: EcoProbSet Product 

Shima Azimi, Christian Massari, Gaia Roati, Silvia Barbetta, and Riccardo Rigon

This study aims at integrating global precipitation data into hydrological models at the catchment scale, a common practice in hydrological research. Specifically, the study investigates how biased spatial and temporal patterns in precipitation data affect model performance and uncertainty. The European Meteorological Observations (EMO) and Climate Hazards Group InfraRed Precipitation with Station data (CHIRPS) global datasets are utilized as inputs for the GEOframe-NewAGE hydrological model to simulate the hydrological processes of the mountainous Aosta Valley catchment in northwestern Italy. Subsequently, the uncertainty of the hydrological model forced with global precipitation data is assessed using a proposed method called Empirical Conditional Probability (EcoProb). The results show that, although traditional performance metrics suggest similar outcomes for the model forced with EMO and CHIRPS, the proposed uncertainty analysis reveals higher uncertainty when CHIRPS is used as the precipitation input. To leverage all useful information in the global precipitation data, the spatial correlation of CHIRPS is combined with a subset of raingauges using the EcoProb method to modify the EMO precipitation data. This approach enables the integration of the advantages of EMO and CHIRPS, which offer higher temporal and spatial correlation with ground observation, respectively, into a unified precipitation product. The combined dataset, referred to as the EcoProbSet product in this study, outperforms both the CHIRPS and EMO products, reducing the uncertainty introduced into hydrological models compared to the original global datasets.

How to cite: Azimi, S., Massari, C., Roati, G., Barbetta, S., and Rigon, R.: A new tool for correcting the spatial and temporal pattern of global precipitation products across mountainous catchments: EcoProbSet Product, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2770, https://doi.org/10.5194/egusphere-egu25-2770, 2025.

EGU25-3254 | ECS | Posters on site | HS7.2

Exploring Hourly Rainfall Extremes in a Changing Climate 

Marc Lennartz and Benjamin Poschlod

Previous research shows that for limited sample sizes applying the simplified metastatistical extreme value (sMEV) distribution instead of the more commonly used general extreme value (GEV) distribution can significantly reduce the associated uncertainty in rainfall return levels. Recent literature has also highlighted the possibility to analyze the effects of climate change using the non-stationary version of the sMEV distribution. Thus, the objective of this study is to test the performance of the sMEV and GEV for hourly precipitation using a convection-permitting regional climate model. The global climate model MIROC5 is employed to drive the regional climate model COSMO over the greater Germany area for the past, near future, and distant future. It is set up at a high temporal and spatial resolution allowing it to explicitly resolve deep convection, which is important when assessing extreme hourly precipitation. No comparable time series from a convection-permitting model has previously been analyzed using the sMEV distribution. The results show that the sMEV performs much better than the GEV in terms of the uncertainty for almost all return periods regardless of the observational years available. In addition, there is a north-south gradient in the return level difference, the uncertainty difference and the adequacy of the left-censoring threshold chosen for the sMEV. Investigating non-stationary versions of the sMEV and GEV shows that the non-stationary sMEV is more suitable to describing the change in return levels. However, both implemented versions of the non-stationary distributions are limited by the complexity of the temperature dependency. Therefore, we recommend a careful application for the prediction of return levels under higher temperatures. 

How to cite: Lennartz, M. and Poschlod, B.: Exploring Hourly Rainfall Extremes in a Changing Climate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3254, https://doi.org/10.5194/egusphere-egu25-3254, 2025.

EGU25-3262 | ECS | Orals | HS7.2

How IDF Relations Changed in the Past and How They Will Change in the Future 

Felix Fauer and Henning Rust

We investigate intensity-duration-frequency (IDF) relations. They describe the major statistical characteristics of extreme precipitation events (return level, return period, time scale) and provide information on the probability of exceedance of certain precipitation intensities. IDF relations help to visualize either how extreme (in terms of probability/frequency/return period) a specific event is or which intensity is expected for a given probability. We model the distribution of extreme precipitation in an extreme-value statistics setting. To increase model efficiency, we include the duration and model a duration-dependent GEV. The durations range from minutes to days and are modeled in one single model in order to prevent quantile-crossing and to assure that estimated quantiles are consistent. This way, we are capable of considering large-scale influences by using covariates for the GEV parameters.

The influence of climate change is included by letting the GEV parameters (covariates) depend on the covariates NAO, temperature, humidity, blocking and year (as a proxy for climate change). We found an increase in probability of extreme precipitation with year and temperature, while the effect of the other variables depends on the season. We present a downscaling approach under the perfect-prognosis assumption as a proof-of-concept, where we use future values of large-scale covariates from climate projections to derive future GEV distributions. This poses some challenges because the polynomial dependencies of the past might not hold for an extrapolation into the future. Right now, our model is based on measurement stations, but we will give an outlook how we plan to include gridded datasets of precipitation observations or reanalyses.

How to cite: Fauer, F. and Rust, H.: How IDF Relations Changed in the Past and How They Will Change in the Future, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3262, https://doi.org/10.5194/egusphere-egu25-3262, 2025.

EGU25-4086 | ECS | Orals | HS7.2

Can discharge be used to inversely correct precipitation? 

Ashish Manoj J, Ralf Loritz, Hoshin Gupta, and Erwin Zehe

This study explores the feasibility of using the information contained in observed streamflow discharge measurements to inversely correct catchment-average precipitation time series provided by reanalysis products. We explore this possibility by training LSTM models to predict precipitation. The first model uses discharge as an input feature along with other meteorological factors, while the second model uses only the meteorological factors. Although the model provided with discharge information showed better mean performance, a detailed analysis of various time series measures across the continental scale revealed underestimation biases when compared with the original reanalysis product used for training. However, an out-of-sample test showed that the inversely estimated precipitation is better able to reproduce small-scale, high-impact events that are poorly represented in the original reanalysis product. Further, using the inversely generated precipitation time series for classical hydrological “forward” modeling resulted in improved estimates for streamflow and soil moisture. Given the notable disconnect between reanalysis products and extreme events, particularly in data-scarce regions worldwide, our findings have implications for achieving better estimates of precipitation associated with high-impact events.

How to cite: Manoj J, A., Loritz, R., Gupta, H., and Zehe, E.: Can discharge be used to inversely correct precipitation?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4086, https://doi.org/10.5194/egusphere-egu25-4086, 2025.

EGU25-4684 | ECS | Orals | HS7.2

Precipitation-driven storm types and their climatology across the Alpine range 

Georgia Papacharalampous, Eleonora Dallan, Moshe Armon, Joydeb Saha, Colin Price, Marco Borga, and Francesco Marra

The separation of storms into physically meaningful classes, including the key distinction between convective and non-convective events, is crucial for advancing precipitation science. Indeed, each of these classes may necessitate different modelling strategies, or distinct bias adjustment procedures for climate model simulations. Here, we present a large-scale study that aimed at achieving this separation only based on information from precipitation timeseries. We focused on a vast set of sub-hourly rain gauge records collected from four countries across the Alpine region and extracted hundreds of thousands of storms. We used an unsupervised clustering algorithm based on a small set of features to organize the storms into storm types. Despite the simplicity of the clustering approach, we successfully distinguished convective storms from other types, as validated using independent features that were not involved in the clustering, such as lightning counts. We analyzed the climatology of the storm types, including investigations of their spatial coherence and temporal changes in their occurrence. Overall, we believe that the storm clusters we provide can be used for several purposes, ranging from developing stochastic models tailored on the storm types of interests to improving bias adjustment methods for climate simulations. Given its simplicity and versatility, the framework can be transferred to other regions globally, with marginal adjustments based on the prior knowledge of the regional climatology and on the research objectives.

Our 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).

How to cite: Papacharalampous, G., Dallan, E., Armon, M., Saha, J., Price, C., Borga, M., and Marra, F.: Precipitation-driven storm types and their climatology across the Alpine range, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4684, https://doi.org/10.5194/egusphere-egu25-4684, 2025.

EGU25-4866 | Orals | HS7.2

Toward the stochastic modelling of extreme precipitation probability with thermodynamic and dynamic covariates 

Francesco Marra, Riccardo Ciceri, Samuele Stante, and Cinzia Sada

To properly adapt to climate change, we need to estimate extreme precipitation probability in future climate scenarios. The task is particularly challenging for sub-daily and sub-hourly extremes, as they are hardly represented by most of the available climate models. As an alternative to explicit model simulations, one can use stochastic models trained on physical covariates. For example, it was recently shown that we can predict changes in sub-daily and sub-hourly extreme precipitation only based on shifts in wet-day daily temperatures. With the aim of extending the applicability of such stochastic models, we examine here the use of covariates representing both thermodynamic and dynamic processes.

We focus on a set of ~300 stations in the Alps (from France, Switzerland, Austria, Italy) for which we have sub-daily precipitation and temperature observations. First, we assess the importance of statistical independence of the events on the identification of the scaling relationships between extreme precipitation and temperature that are commonly used to quantify the thermodynamic component. Then, we evaluate the relative importance of the thermodynamic and dynamic components for durations ranging between 10 minutes and 24 hours using as covariates dew point, vertical velocity at 500 hPa, and divergence at 300 hPa from ERA5 reanalysis simulations.

Our results show that (1) evaluating extreme precipitation-temperature scaling relations using all the wet time intervals (as done in several studies) leads to biased estimates of the scaling rates relevant for extreme sub-daily precipitation projections. (2) The scaling rates between extreme precipitation and dew point tend to decrease logarithmically with duration, an information that can be used to extract the scaling rate at sub-hourly durations from hourly observations. (3) The importance of the thermodynamic component decreases with duration (rank correlation decreases from ~0.55 at 10 minutes to ~0.2 at 24 hours), while the importance of the dynamic component that can be appreciated at the ERA5 resolution (~30 km) tends to increase with duration (rank correlation increases from ~0.2 at 10 minutes to ~0.45 at 24 hours). (4) From a stochastic simulation perspective, temperatures and dew point during precipitation events in the Alps can be simulated using generalized normal distributions (or normal distributions in case of seasonal data), while vertical velocities and divergence need to be simulated using skewed models such as a generalized extreme value distribution. 

How to cite: Marra, F., Ciceri, R., Stante, S., and Sada, C.: Toward the stochastic modelling of extreme precipitation probability with thermodynamic and dynamic covariates, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4866, https://doi.org/10.5194/egusphere-egu25-4866, 2025.

EGU25-5084 | ECS | Orals | HS7.2

Development of Rainfall Scenario with Transition Probability Reflecting on Temporal Distribution of Heavy Rainstorm Events 

Hoyoung Cha, Jongjin Baik, Jinwook Lee, Wooyoung Na, and Changhyun Jun

  This study proposes a method utilizing Rainfall Transition Probability (RTP) to create rainfall scenarios that consider the temporal distribution of heavy rainstorm events. RTP refers to the probability of rainfall amount at time t occurring after a specific rainfall amount at time t+1. The method consists of a temporal distribution that builds region-specific RTPs using rainfall data observed at 1-minute interval, a function that users define the desired conditions for the rainfall scenario, and a processing module that generates scenarios based on the RTP. To develop the RTP, the rainfall data about 1-minute interval used for separating Independent Rainstorm Events (IREs) according to each region. Among the identified IREs, those exhibiting high-intensity rainfall (above 15 mm/hour) are used to calculate and establish the RTP. Afterward, users define the conditions for the rainfall scenario in the function with conditions such as region, total rainfall, and rainfall duration. The generator then utilizes the RTP for the selected region to generate various rainfall scenarios with different temporal distributions and presents them to the user. By extracting the temporal distribution from regional IREs, the generator reflects local rainfall patterns and can be applied to regional hydrological modelling.

Keywords: Rainfall Generator, Rainfall Transition Probability, 1-minute Rainfall Data, Temporal Distribution, Heavy Rainstorm Events

 

Acknowledgment

This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (RS-2024-00334564).

 

How to cite: Cha, H., Baik, J., Lee, J., Na, W., and Jun, C.: Development of Rainfall Scenario with Transition Probability Reflecting on Temporal Distribution of Heavy Rainstorm Events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5084, https://doi.org/10.5194/egusphere-egu25-5084, 2025.

Abstract

In this study was investigated three different microphysics schemes on the rainfall patterns over Kuwait on 02 January 2022. The primary objective is to improve precipitation predictions using the Weather Research and Forecasting (WRF) high resolution 4 km model, which has been dynamically downscaled from the Community Climate Model version 4 (CCM4). The performance of three selected microphysics schemes—Lin, WSM6, and Thompson was evaluated using the ERA5 reanalysis dataset. ERA5 has been previously validated in this region and has consistently provided reliable results, making it a suitable dataset for such studies. Three numerical simulations were conducted using the WRF model, each incorporating one of the three microphysics schemes. The simulations were assessed by comparing the model outputs against the ERA5 data to determine the accuracy of the rainfall forecasts. The results revealed that the WRF Single-Moment 6-class microphysics scheme (WSM6) outperformed the other microphysics schemes, including Lin and Thompson, in forecasting rainfall patterns during the storm. The Lin scheme was found to be the least reliable, providing less accurate rainfall predictions compared to the Thompson and WSM6 schemes. This study highlights the critical role of selecting appropriate microphysics schemes for accurate precipitation prediction, particularly in extreme weather events like the 2022 storm in Kuwait. The findings suggest that the WSM6 scheme is a more effective choice for rainfall forecasting in this region, whereas the Lin scheme may not be as suitable for this particular type of storm event. Further research is recommended to extend this analysis to different regions and storms for more comprehensive results.

How to cite: Alsarraf, H.: Evaluation of WRF Microphysics Schemes for Precipitation Forecasting in an Arid Region: A Case Study Over Kuwait, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5123, https://doi.org/10.5194/egusphere-egu25-5123, 2025.

EGU25-6812 | ECS | Orals | HS7.2

Comparison and evaluation of different precipitation products in capturing climate extremes in Kamp Catchment, Austria 

Zryab Babker, Morteza Zagar, Tim G. Reichenau, Mohammed Basheer, and Karl Schneider

The availability of accurate long-term gap-free precipitation data at high spatiotemporal resolutions is crucial for hydroclimatic extremes assessment, water resources management, infrastructure design, hydrological modeling, and evaluation of climate change impacts. However, many ground precipitation data contain gaps, which can hinder accurate assessments and analyses. Therefore, different gridded precipitation products (PPs) are promising alternatives to overcome this deficiency, especially in heterogeneous regions with different terrains where ground observations are sparse or non-existent. This study evaluates four daily precipitation products, i.e., SPARTACUS, IMERG-V07, CHIRPS-V2.0, and ERA5-land, to determine their performance in representing observed patterns, the intensity, and frequency of extreme precipitation events in Kamp Catchment in Austria for the period 1998-2020 at different temporal scales. The Kamp River is the longest in the “Waldviertel” region and has key ecological, societal, and economic functions, with many popular leisure and excursion destinations for tourism. The catchment also frequently experiences severe floods, causing adverse socioeconomic impacts. Ground-based precipitation data from 33 stations distributed within and around the catchment are used to conduct point-to-pixel evaluation for the four products. To measure the disparity between the products and the ground observations, six performance metrics were used: the Root Mean Square Error (RMSE), Mean Absolute Error (MAE), Mean Bias Error (MBE), Nash-Sutcliffe Efficiency (NSE), Correlation coefficient (r), and Willmott index of agreement (d). The intensity and frequency of extreme precipitation reflected by the four evaluated PPs are assessed using selected extreme climate indices defined by the Expert Team on Climate Change Detection and Indices (ETCCDI). The PPs were ranked to select the best-performing product in the study area. The ranking results of the performance metrics revealed that SPARTACUS is the top-performing product on a daily and monthly scale and in capturing the frequency and intensity of precipitation extremes, followed by IMERG-V07 and ERA5-land, whereas CHIRPS-V2.0 ranked the lowest. SPARTACUS showed superior performance across the catchment with the highest correlation with the observed data and lowest bias (on daily and monthly scales, mean r values are 0.92 and 0.96 and mean MBE values are -0.02 and -0.81, respectively). Other products exhibit systematic precipitation underestimation. Regarding capturing precipitation extremes, all products show low skills and overestimate the daily extreme precipitation events, with the highest NSE of -0.32 shown in SPARTACUS. CHIRPS-V2.0 and ERA5-land presented different performances for detecting the longest wet and dry spells in the catchment. CHIRPS-V2.0 overestimated the consecutive dry days (CDD) and underestimated the consecutive wet days (CWD), whereas ERA5-land shows the opposite pattern. SPARTACUS shows minor overestimation of CDD and underestimation of CWD (MBE = -0.09 and 0.13 mm, respectively). Accordingly, a simple drought assessment was performed in the catchment using SPARTACUS data and the Standardized Precipitation Index (SPI). Our results highlight the importance of site-specific validation before using any precipitation products.

This study is conducted within the frame of the DISTENDER project (EU Horizon-ID 101056836), where climate extremes and climate change impacts upon several European catchments are analyzed and robust adaptation strategies are developed.

 

Keywords: Precipitation extremes, Precipitation products, Point-to-pixel evaluation, SPI, Kamp catchment, Austria

How to cite: Babker, Z., Zagar, M., G. Reichenau, T., Basheer, M., and Schneider, K.: Comparison and evaluation of different precipitation products in capturing climate extremes in Kamp Catchment, Austria, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6812, https://doi.org/10.5194/egusphere-egu25-6812, 2025.

EGU25-7599 | ECS | Orals | HS7.2

Prior knowledge-constrained deep learning for probabilistic precipitation downscaling 

Dayang Li, Long Yang, Baoxiang Pan, Yuan Liu, and Yan Zhou

Precipitation downscaling, particularly at convection-permitting scales (less than 4 km), is highly uncertain. This is especially pronounced in mountainous regions due to the interplay of complex topography and atmospheric dynamics. It impedes reliable estimation of variability and risks in localized extreme rainstorms. Deep learning-based downscaling methods have gained increasing attention but have primarily focused on deterministic prediction, which fails to capture uncertainty. Here we developed a novel Probabilistic High-resolution Precipitation Downscaling Network (P-HRDNet) with prior knowledge of key precipitation characteristics to design its loss function and model architecture. This knowledge includes data imbalance, skewed distribution, heteroscedasticity, and spatial and temporal dependencies of precipitation. P-HRDNet was tested in the southeastern Tibetan Plateau, a mountainous region lacking high-resolution precipitation data. Ten-year WRF simulations with nested domains provided coarse (9 km) and fine resolution (1 km) daily precipitation to train P-HRDNet. Compared with a baseline model SRCNN, P-HRDNet achieved greater accuracy in terms of root mean square error, mean absolute error, and Pearson correlation coefficient. Besides, it offers better uncertainty coverage and narrower uncertainty widths. This superiority is particularly evident in the extreme values. Our study highlights the importance of incorporating prior knowledge of precipitation characteristics into deep learning, and has a potential to physically constrain Artitifical-Intelligience (AI) based weather forecasting models. Furthermore, our WRF-AI framework offers an efficient solution for obtaining reliable high-resolution precipitation estimates in poorly gauged regions.

How to cite: Li, D., Yang, L., Pan, B., Liu, Y., and Zhou, Y.: Prior knowledge-constrained deep learning for probabilistic precipitation downscaling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7599, https://doi.org/10.5194/egusphere-egu25-7599, 2025.

Summer precipitation over High Mountain Asia (HMA) has exhibited a dipolar trend over the past 50 years. Understanding its future changes and underlying mechanisms relies heavily on climate models. However, the impact and mechanisms of model resolution on the simulation of long-term precipitation trends over the HMA remain underexplored. In this study, we use six pairs of models with high- and low-resolution comparisons from the CMIP6 all-forcing experiments to investigate the resolution-dependent differences in the long-term trends of summer precipitation from 1951 to 2024. The results show that compared to low-resolution models, the simulations from high-resolution models are closer to observations, with the largest improvement in the southern margin of the HMA and surrounding areas (STP), where the wet bias is reduced by approximately 65%.  The moisture budget, moist static energy budget, and mixed-layer heat budget are used to explore the mechanism behind this reduction in wet bias. High-resolution models, with their enhanced ability to simulate oceanic advection and mixing, can capture the central-warm and eastern-cool tropical Indian Ocean SST pattern better. This SST pattern suppresses precipitation over Malaysia and the South China Sea, triggering Rossby waves that generate an anomalous anticyclone over the northern Bay of Bengal. The anticyclone then transports dry air to the STP, suppressing local convection and reducing wet bias. Our study emphasizes the importance of simulating Indian Ocean warming for accurately representing long-term precipitation trends over HMA.

How to cite: li, L.: Precipitation Trends over southern High Mountain Asia affected by Indian Ocean warming: Insights from high- and low-resolution versions of CMIP6 models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7737, https://doi.org/10.5194/egusphere-egu25-7737, 2025.

EGU25-7792 | Posters on site | HS7.2

Statistical downscaling of hourly precipitation in South Korea using the MS-PRISM method 

Maeng-Ki Kim, Sang Jeong, and Youngseok Lee

In this study, we developed a grid climate dataset with a horizontal resolution of 500m × 500m for South Korea, utilizing observational station data from the Korea Meteorological Administration (KMA). The high-resolution 500m data were calculated using a newly developed Multi-Step (MS) PRISM (Parameter-elevation Regressions on Independent Slopes Model) method, which enhances the Modified Korean (MK) PRISM—a statistical downscaling technique for estimating high-resolution gridded data from observational data. First, to produce high-resolution hourly precipitation data, we performed quality control on the hourly precipitation observation data to select valid entries. Next, we created geographic information data, including Digital Elevation Model (DEM), aspect, and coastal proximity, all at a resolution of 500m. This geographic data was then applied to the MS-PRISM method to calculate hourly precipitation data at the same resolution. To confirm the reliability of the 500m resolution hourly precipitation produced, we conducted a verification of the final estimated data. We compared and analyzed the daily precipitation estimation errors as well as the hourly precipitation estimation errors at the same spatial resolution. Additionally, we evaluated the estimation results based on changes in spatiotemporal resolution by comparing the estimation errors associated with different spatial resolutions while maintaining the same temporal resolution.

How to cite: Kim, M.-K., Jeong, S., and Lee, Y.: Statistical downscaling of hourly precipitation in South Korea using the MS-PRISM method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7792, https://doi.org/10.5194/egusphere-egu25-7792, 2025.

EGU25-8629 | ECS | Orals | HS7.2

Correction of Precipitation Bias from Convection-Permitting Models at the Station Scale in Switzerland 

Lauren Cook, Trang Nguyen, Andreas Dietzel, and Patricio Velasquez

Unlike regional climate models, convection-permitting models (CPMs) are able to resolve convection-scale processes and therefore better estimate short-duration, extreme precipitation events, particularly useful for the urban drainage community. Despite their state-of-the-art capabilities, bias correction of CPMs is still required to ensure their output is representative of the station scale, a resolution needed by many urban drainage models. Due to its simplicity, quantile-mapping is commonly used for bias-correction and downscaling, but does come with limitations that have not yet been evaluated for CPMs. This study tests five variations of empirical quantile-mapping to bias-correct and downscale the 2.2 km simulations of COSMO-CLM (a CPM) for over 70 weather stations in Switzerland. Ten years of simulation data are corrected using ten years of observations at the 30-minute interval. Traditional QM and several advanced versions are evaluated, including: using a 91-day moving window to account for temporal variability, spatial pooling of surrounding grid cells for spatial variability, and extending the observational record (to 30 years) for data variability. These techniques are validated using cross-validation and through evaluation of historical rainfall indices (e.g., consecutive dry days) and the climate change signal. Findings show that wet biases in raw CPM output remain (up to 30-35 mm/hour above the 98th quantile) and only the moving window technique (and its combination with spatial pooling) is able to reduce biases in quantiles above the 98th. All QM methods do reduce remaining biases, but can distort the climate change signal, particularly in indices related to frequency of rainfall. Despite the additional computational burden, the moving window technique is highly recommended to the urban drainage community as a robust technique for CPM downscaling. As more CPM simulations become available, future work will reexamine these aspects for a range of CPMs, time periods, and simulation domains.

How to cite: Cook, L., Nguyen, T., Dietzel, A., and Velasquez, P.: Correction of Precipitation Bias from Convection-Permitting Models at the Station Scale in Switzerland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8629, https://doi.org/10.5194/egusphere-egu25-8629, 2025.

EGU25-9341 | ECS | Orals | HS7.2

Decadal climatology and trends in global oceanic precipitation from 27 satellite and reanalysis datasets 

Si Cheng, Lisa Alexander, and Steven Sherwood

Understanding changes in global oceanic precipitation remains challenging due to limitations in current observational datasets and model deficiencies, particularly in the representation of cloud and precipitation properties within oceanic regions. To address this, we examined climatologies and trends in oceanic precipitation between 2001 and 2020 using a collection of 27 state-of-the-art satellite and reanalysis datasets available on a uniform daily 1°×1° resolution from the Frequent Rainfall Observations on Grids (FROGS) database. The results showed that reanalysis datasets generally report higher annual mean daily precipitation than satellite datasets. The tropical region exhibits the greatest absolute discrepancies in precipitation rates, while arid regions such as the southeast Pacific and Atlantic show significant relative differences among products. An increasing trend is primarily observed in satellite products, whereas reanalyses suggest strong declines. Taken together, reanalyses show pronounced decreases over the Intertropical Convergence Zone (ITCZ) and North Atlantic, contradicting the “wet gets wetter, dry gets drier” (WWDD) pattern. In contrast, the satellites better align with the WWDD pattern, with over half of oceanic regions meeting this expectation. The precipitation trend in the combined reanalysis products also exhibits the weakest consistency with sea surface temperature (SST) trends in wet regions (34.2%), compared with dry regions in the reanalysis cluster (53.4%) and both wet (59.6%) and dry (58.5%) regions in the satellite cluster. We recommend using an ensemble of satellite products for investigating global oceanic precipitation while exercising greater caution when utilizing reanalysis datasets.

How to cite: Cheng, S., Alexander, L., and Sherwood, S.: Decadal climatology and trends in global oceanic precipitation from 27 satellite and reanalysis datasets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9341, https://doi.org/10.5194/egusphere-egu25-9341, 2025.

EGU25-9859 | ECS | Posters on site | HS7.2

Drizzle Bias adjustment in climate models: A simple two-step downscaling approach 

Matteo Sangiorgio, Roberto Caspani, Lorenzo Scarpellini, Matteo Giuliani, and Andrea Castelletti

Precipitation is a key variable for assessing the impacts of climate change across diverse sectors, from hydrology to ecology. However, climate models frequently overestimate the occurrence of light precipitation events—days or hours that should be dry are instead assigned a low rainfall rate. This pervasive issue, known as the “drizzle bias” or “drizzle problem” in climate science, undermines the reliability of climate impact assessments.

Traditional bias correction methods, such as linear scaling or empirical quantile mapping, address overall precipitation distributions but often fail to properly account for the frequency and duration of wet and dry periods. As a result, these methods may improve precipitation totals but fail to correct the skewed distribution of rainy events.

In this study, we propose a simple yet effective two-step statistical downscaling approach to address the drizzle bias. The first step aligns the frequency of wet and dry periods by assuming equivalence between observed and simulated rain frequencies. The second step corrects the precipitation distribution exclusively for wet samples.

We apply this methodology to a range of climate data products, including ERA5 Land reanalyses, as well as simulations from global circulation models (GCMs), regional circulation models (RCMs), and convection-permitting models (CPMs). Our analysis focuses on multiple measurement stations in Northern Italy, encompassing urban contexts such as Milan and mountainous contexts in the Italian Alps. Results reveal that drizzle bias is a widespread issue across these datasets, regardless of the modeling framework.

The findings demonstrate that our two-step downscaling approach effectively adjusts for drizzle bias, significantly improving the statistical fidelity of precipitation projections. This approach offers a straightforward and practical solution for enhancing the reliability of climate model outputs, enabling more robust assessments of climate change impacts across sectors sensitive to precipitation variability.

How to cite: Sangiorgio, M., Caspani, R., Scarpellini, L., Giuliani, M., and Castelletti, A.: Drizzle Bias adjustment in climate models: A simple two-step downscaling approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9859, https://doi.org/10.5194/egusphere-egu25-9859, 2025.

EGU25-10165 | ECS | Posters on site | HS7.2

Removal of interfering RLAN signals from C-band weather radar data 

Krystian Specht, Katarzyna Ośródka, Jan Szturc, and Włodzimierz Freda

The algorithm of removing interfering RLAN signals (so called spikes) in weather radar data is implemented in the Institute of Meteorology and Water Management – National Research Institute (IMGW) as a component of the RADVOL-QC system for the radar data quality control. Eliminating the interfering signals in C-band (5 GHz) radars is important for accurate weather monitoring. The main difficulty in spike removal are their unique shapes, and the task is especially challenging while they overlap the precipitation.

The process of detecting interference caused by signals from the RLAN network is carried out by evaluating the variability of echoes along and across the beam for each bin at various elevation angles. Such echoes are considered potential spikes. For each azimuth, the number of bins containing potential spike echoes is determined. If this count exceeds the established threshold for a given azimuth, the echoes are treated as real spikes.

The spike correction process consists of analyzing each bin with detected real spike and its surroundings. The analysis extends to bins in adjacent and further azimuths on left and right until bins without detected spikes are encountered. Depending on the specific case, these echoes may be replaced with an arithmetic mean if classified as precipitation or removed entirely. While removing spikes, the analysis extends to adjacent azimuths within a range of 3 to 4 bins on either side to ensure accurate identification and removal of false echoes. This extended analysis considers potential anomalies in adjacent data that may have been overlooked during the detection process.

Examples of applied techniques are presented using the weather radar product maximum reflectivity (CMAX). The examples illustrate the enhancement of the radar data, where the extended analysis effectively eliminates RLAN interference that was not identified by the detection algorithm but falls within the analysis area. This improvement is crucial from a meteorological perspective, as high-quality radar data significantly impacts meteorological and hydrological models, leading to more accurate forecasts.

How to cite: Specht, K., Ośródka, K., Szturc, J., and Freda, W.: Removal of interfering RLAN signals from C-band weather radar data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10165, https://doi.org/10.5194/egusphere-egu25-10165, 2025.

The increasing frequency and intensity of extreme events due to global warming, such as heavy rainfall and consequent floods, underline the need for research on the driving factors of these extremes. Accurate simulations of meteorological extremes at convection-permitting scale are crucial for understanding their spatial and temporal characteristics. Recently, various studies have demonstrated the added value of using convection-permitting regional climate models to simulate extreme precipitation. Further improvements of these regional models can therefore lay the foundation for better impact assessment, as well as for developing adaptation measures to tackle climate change. 

In this study, we investigate the optimal model configuration for the regional climate model REMO2020-iMOVE to capture extreme precipitation events, using the heavy rainfall that led to the devastating Ahr valley flood of July 2021 as a case study. Our simulations are performed with the non-hydrostatic version of REMO with ERA5 reanalysis data as forcing at a horizontal resolution of 3 km. By including the vegetation module iMOVE, we aim to improve the representation of vegetation-atmosphere interactions and, in a future step, investigate the effects of land use and land cover changes on extreme events. Here, we explore the impact of different model setups such as different domain sizes and initialization times on the simulation results. Furthermore, we validate our findings against observations and assess uncertainty within the model. This research provides insight into optimizing regional climate models to improve our understanding of extreme weather events. 

How to cite: Detjen, L., Rechid, D., and Böhner, J.: Optimizing convection-permitting model configurations for accurate simulation of extreme precipitation events with the regional climate model REMO-iMOVE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11604, https://doi.org/10.5194/egusphere-egu25-11604, 2025.

EGU25-12783 | Orals | HS7.2

Using LOCA to downscale precipitation over Europe 

Bridget Thrasher

Localized Constructed Analogs (LOCA) is a statistical downscaling technique that uses a multiple scale approach to determine appropriate local analogs from historical data. It was developed with a particular focus on the preservation of extreme events that were dampened or lost altogether when employing earlier analog methods. The LOCA method has been used to produce relatively high-resolution projections of precipitation over the coterminous United States for use in hydrologic applications but has never been applied over Europe. In this presentation we will describe the method in detail and show how it is being utilized to downscale CMIP6 precipitation to 1 arcmin x 1 arcmin horizontal resolution over the continent using the European Meteorological Observations (EMO-1) gridded dataset as the analog pool. Lastly, we will compare the LOCA output to that from other downscaled products. 

How to cite: Thrasher, B.: Using LOCA to downscale precipitation over Europe, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12783, https://doi.org/10.5194/egusphere-egu25-12783, 2025.

EGU25-12929 | ECS | Posters on site | HS7.2

Reanalysis Data in Hydrological Applications: A Case Study from Georgia 

Andrea Nobile, Francesca Zanello, Francesco Lubrano, Matteo Nicolini, and Elisa Arnone

Reanalysis data have proven to be a valuable support for hydrologic modeling and calculation of standardized climate indices, useful tools for characterizing local climate regimes and improving water resource management in areas with limited availability of observational data.

This study examines the use of ERA5 dataset emphasizing bias correction techniques to enhance their applicability and understanding their limits in a case study in Georgia. The work assesses the effectiveness of five bias correction techniques - Linear Scaling (LS), Empirical Quantile Mapping (QM-EMP), Quantile Mapping Spline Bias Correction (QM-SBC), Mean Bias Subtraction (MBS), and Simple Linear Regression (SLR) - each examined through two different bias correction approaches: classical and sliding window, applied to daily and monthly reanalysis time series. Observational climate data are scarce in Georgia, therefore the opportunity of using reanalysis data for hydrological studies is of great interest for engineering applications.

In this study, performed in collaboration with Idrostudi S.r.l., one of the foremost European engineering professional services consulting firms, the extraction of ERA5 data for the entire nation of Georgia was performed automatically by developed algorithms that also allowed to do bias correction. The algorithms, developed using the open-source programming language R, employ observed data collected by five meteorological stations across diverse climatic zones of Georgia to test and compare different bias correction methodologies. The aim is to validate the performance of bias correction methods to improve the accuracy of rainfall data generated by ERA5 reanalysis model at daily and monthly scales. The techniques were evaluated carrying out two experiments, i.e. using (i) the complete datasets and (ii) the series that were split into a calibration and validation subset; metrics such as Root Mean Square Error (RMSE) and Nash-Sutcliffe Efficiency (NSE) were used to assess the performance. The dataset undergoes a calibration phase using 70% of the data to tune the bias correction methods, followed by a validation phase with the remaining 30% to test their effectiveness.

Results demonstrate that bias correction improves the quality of reanalysis data, dealing to enhanced reliability for hydrological modelling and climate index computation. The LS method has emerged as the most effective among classical techniques for bias correction in daily-scale reanalysis data when all data are available. The introduction of the Sliding Window approach has further enhanced the performance of all techniques, adapting the correction to local variations and improving accuracy for daily precipitation events. It is important to note, however, that at a monthly scale, the classic approach to bias correction already proves to be sufficiently reliable. Therefore, further enhancements through the sliding window approach are not deemed necessary for monthly corrections. In the experiment (ii), techniques such as QM-EMP, QM-SBC, and SLR proved to be more suitable for applications in climatic contexts with high variability and fragmentation. This underlines the importance of selecting the appropriate bias correction technique based on the quality and availability of data, as well as the specific objectives of the analysis. Further studies are needed for a further optimization of bias correction approaches.

How to cite: Nobile, A., Zanello, F., Lubrano, F., Nicolini, M., and Arnone, E.: Reanalysis Data in Hydrological Applications: A Case Study from Georgia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12929, https://doi.org/10.5194/egusphere-egu25-12929, 2025.

EGU25-13830 | Posters on site | HS7.2

Considerations in multifractal downscaling of rainfall: canonical vs. microcanonical cascades 

Alin Andrei Carsteanu, Stergios Emmanouil, Andreas Langousis, and Roberto Deidda

Disaggregation of rainfall time series focuses on preserving the statistical properties of those small-scale intensities, which are being downscaled from measured large-scale values. Multifractal scaling properties have offered, for a few decades already, a parsimonious framework for simulating the joint statistics observed in the small-scale values, and recent work emphasizes the use of more sophisticated cascading processes, in order to better capture all statistical requirements imposed (Cappelli et al., Stoch Environ Res Risk Assess 2024, https://doi.org/10.1007/s00477-024-02827-8). Comparisons between downscaling models based on canonical vs. microcanonical cascades have been presented already more than two decades ago (see e.g. Molnar and Burlando, Atmos Res 77, 2005, https://doi.org/10.1016/j.atmosres.2004.10.024), but recent theoretical results (Aguilar-Flores and Carsteanu, Fractals 32, 2024, https://doi.org/10.1142/S0218348X24500725) have prompted us to consider the importance of taking into account the asymptotic properties of the measures generated by canonical and microcanonical cascades, respectively, for downscaling purposes. The reflection of such properties in real-life rainfall data is being analyzed in the work communicated herein.

How to cite: Carsteanu, A. A., Emmanouil, S., Langousis, A., and Deidda, R.: Considerations in multifractal downscaling of rainfall: canonical vs. microcanonical cascades, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13830, https://doi.org/10.5194/egusphere-egu25-13830, 2025.

EGU25-13869 | Posters on site | HS7.2

MET Nordic Reanalysis data improves the performance of catchment-level hydrological models 

Csilla Farkas, Moritz Shore, Jessica Fennell, and Mojtaba Shafiei

High-quality input data is the foundation for good model performance, including catchment level hydrological models. The resolution and quality of meteorological data has a direct impact on modelling results and as such strongly influences the outcomes of scenario analyses of different types. Nowadays one can choose between different meteorological products when setting up a mathematical model, including direct measurements and reanalyses. The goal of this study was to test the ability of MET Nordic data, a reanalysis product from Met Norway, on improving the simulations of hydrological models.  The MET Nordic Reanalysis Dataset consists of post-processed products that (a) describe the current and past weather (reanalysis), and (b) gives a best estimate of the weather in the short-term future (forecasts). The products integrate output from MetCoOp Ensemble Prediction System (MEPS) as well as measurements from various observational sources, including crowdsourced weather stations. 

Two different catchment models were set up and calibrated against measured discharge data. The SWAT+ model was applied in two Norwegian and one Danish catchment, while the CWatM model was tested in one Norwegian catchment. The model’s performance was compared when using input datasets from measuring stations and MET Nordic reanalysis data. We concluded that applying reanalysis data can significantly improve the performance of the tested models, therefore the use of these data in hydrological modelling is highly recommended.  

How to cite: Farkas, C., Shore, M., Fennell, J., and Shafiei, M.: MET Nordic Reanalysis data improves the performance of catchment-level hydrological models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13869, https://doi.org/10.5194/egusphere-egu25-13869, 2025.

Probabilistic radar-based precipitation nowcasting has become increasingly crucial for real-time hydrological applications due to its high accuracy at short lead time. However, its reliability for hydrological usage is limited by two major sources of error and uncertainty, both of which tend to exacerbate quickly with lead time. The first source lies in the limitations of nowcasting algorithms, including inaccuracies in rainfield advection and inadequate modeling of rain cell evolution. The second arises from discrepancies in precipitation measurements, referring to the differences between radar-derived estimates and rain gauge observations. Aligning these estimates with actual ground-level precipitation is vital for practical hydrological applications.

This study focuses on addressing the errors and uncertainties inherent in precipitation 'measurements', aiming to enhance the reliability of original nowcasts. Here, uncertainty refers to the range within which the true value is expected to fall at a given confidence level, while error denotes to the systematic bias between estimated and true values. The proposed methodologies utilise rain gauge data as the ground truth and employs the Short-Term Ensemble Prediction System (STEPS) to generate radar-based ensemble nowcasts. To deal with these issues, an initial attempt was conducted with the Censored Shifted Gamma Distribution (CSGD) model. However, the model faces challenges in selecting an appropriate metric as the adjusted value, limiting the potential reduction in RMSE to approximately 5–10%. To overcome this limitation, a random forest (RF) regression model is proposed, as it can avoid predefined assumptions about rainfall intensity distribution. This model incorporates variables such as nowcasted rainfall intensity, orographic features, and meteorological parameters such as wind speed, wind direction, humidity, cloud type, and cloud base height (CBH), to estimate corresponding rain gauge measurements. At each rain gauge location, the error distribution is parametrised by comparing the original and adjusted rainfall intensities and fitting them to various probability functions. These parameters are then spatially interpolated using geostatistical techniques to generate an error map. The resulting error map is applied to correct the original nowcasts across the study area, enhancing their overall accuracy and reliability.

The United Kingdom, benefiting from its comprehensive and high-quality meteorological data, was selected as the study area. The 1-km UK C-band radar composite, derived from the Met Office Nimrod System, serve as the radar rainfall dataset for generating ensemble nowcasts. Rain gauge data and additional meteorological variables are sourced from the Met Office Integrated Data Archive System (MIDAS) and the Met Office LIDARNET ceilometer network. Rainfall events from 2016 to 2022 are analysed, with events from 2016 to 2020 designated as the training period for developing random forest models and error maps. For validation, 20 events from 2021 to 2022 are selected to assess the performance of both the original and adjusted nowcasts. Preliminary results indicate that the adjusted ensemble nowcasts exhibit significantly improved alignment with rain gauge measurements compared to the original nowcasts. These findings highlight the potential of the proposed methodology to reduce both error and uncertainty in radar-based precipitation nowcasting, particularly for hydrological applications such as flood and landslide forecasting.

How to cite: Lin, H.-M. and Wang, L.-P.: Enhancing the applicability of radar-based precipitation nowcasting to hydrological applications with a machine-learning based error modelling method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14377, https://doi.org/10.5194/egusphere-egu25-14377, 2025.

EGU25-14564 | ECS | Posters on site | HS7.2

Blunt Extension and Dynamic Generation of Multifractal Cascade Fields Tree for Rainfall Drop Trajectories Simulations 

Chi-Ling Wei, Auguste Gires, and Li-Pen Wang

Precipitation variability at small space-time scales significantly influences hydrological processes, particularly in heterogeneous environments such as urban areas. Building on established methodologies for generating universal multifractal cascade fields, we propose an alternative approach that optimizes memory efficiency while maintaining the fidelity and flexibility of high-resolution simulations. Our method generates cascade fields dynamically, we call it Cascade Tree, which reduces memory usage by over 100 times compared to precomputing and storing full datasets. This improvement complements existing techniques by offering a scalable option for real-time applications.

 

To further enhance the realism of the simulated fields, we integrate the blunt extension of universal multifractals, which smooths transitions between far branches in Cascade Tree and addresses non-conservativeness in a computationally efficient manner. By leveraging GPU acceleration, we achieve rapid computation of cascade fields, enabling their use in simulating complex phenomena such as rainfall dynamics in turbulent wind fields.

 

The method is applied to simulate 3D trajectories and velocities of raindrops in a high-resolution multifractal turbulent wind field, using real wind field data to improve the applicability of the results. Our simulations capture the spatial and temporal variability of rainfall and demonstrate the dispersion of over 100,000 raindrops across scales relevant to radar pixels and urban catchment hydrology.

 

This work provides new tools for exploring rainfall-driven processes, with applications ranging from downscaling radar precipitation data to refining hydrological response models. By complementing established methods with a memory-efficient and GPU-accelerated framework, our approach bridges the gap between drop-scale dynamics and catchment-scale impacts.

How to cite: Wei, C.-L., Gires, A., and Wang, L.-P.: Blunt Extension and Dynamic Generation of Multifractal Cascade Fields Tree for Rainfall Drop Trajectories Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14564, https://doi.org/10.5194/egusphere-egu25-14564, 2025.

EGU25-14679 | ECS | Orals | HS7.2

Bartlett-Lewis based stochastic rainfall model: An improvement to effectively reproduce sub-hourly rainfall extremes 

Chi Vuong Tai, Jeongha Park, Li-Pen Wang, and Dongkyun Kim

Despite significant advancements in the Poisson cluster-based Bartlett-Lewis model for effectively reproducing rainfall extremes, there is still room for further refinement. This study proposes a refined model, referred to as RBL7, introducing module k with a modified equation for rainfall disaggregation. This adjustment allows the power of the sine function to vary inversely with rain cell duration, thereby capturing the realistic characteristics of rainfall extremes, which often come with high intensity over short durations. Furthermore, an improved calibration approach is also proposed for the first module of the RBL7 model. This involves a hybrid optimization technique combining Particle Swarm Optimization (PSO) and fmincon methods, iterately executed until the objective function reaches the pre-assigned threshold. While the calibration of the RBL7 model relies solely on observed rainfall aggregated at hourly and longer timescales, it effectively reproduces rainfall extremes from uncalibrated sub-hourly to supra-hourly aggregation intervals, outperforming existing models using sine-2 and rectangular pulse shapes. Additionally, this refined model maintains its capability to capture rainfall standard statistics, i.e., mean, variance, covariance, skewness, and proportion of wet period, at various timescales ranging from 5 minutes to a month. These findings highlight the robustness of the RBL7 model in simulating rainfall characteristics, especially extreme values at sub-hourly aggregation intervals.

 

Acknowledgement

This study was supported by Korea Environment Industry & Technology Institute (KEITI) through R&D Program for Innovative Flood Protection Technologies against Climate Crisis Program (or Project), funded by Korea Ministry of Environment(MOE)(RS-2023-00218873).

How to cite: Vuong Tai, C., Park, J., Wang, L.-P., and Kim, D.: Bartlett-Lewis based stochastic rainfall model: An improvement to effectively reproduce sub-hourly rainfall extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14679, https://doi.org/10.5194/egusphere-egu25-14679, 2025.

EGU25-14931 | ECS | Posters on site | HS7.2

Quantifying Future Shifts in Intensity–Duration–Frequency (IDF) in Singapore: A comparison of methods 

Mengzhu Chen, Nadav Peleg, and Simone Fatichi

Intensity-Duration-Frequency (IDF) curves are critical for urban drainage design and flood risk mitigation, particularly in highly urbanized regions like Singapore, where short-duration extreme rainfall events pose significant challenges. This study quantifies future changes in IDF curves and their associated uncertainties under two representative emission scenarios: SSP 2-4.5 and SSP 5-8.5. To construct future IDF curves, we compare two methods. First, we use a stochastic downscaling methodology that makes use of the AWE-GEN weather generator, to downscale precipitation projections from 25 Global Climate Models (GCMs) to the local point scale. The results show that the magnitude of future extreme precipitation quantiles is expected to get higher toward the end of the 21st century under both future scenarios. Higher-emission scenarios lead to substantial intensification of rare precipitation events, accompanied by a large uncertainty. However, internal climate variability is the dominant source of uncertainty, with climate model and emission scenario uncertainties being less relevant. Second, the results are compared with outputs of the TENAX (Temperature dependent Non-Asymptotic statistical model for eXtreme return levels) model, a novel framework that incorporates temperature as a covariate in a physically consistent manner to project rainfall return levels in a warmer climate using fewer inputs. This study compares state-of-the-art methodologies for computing IDF representative of future climates and provides actionable insights for engineers and policymakers to update urban stormwater design guidelines and enhance resilience against future rainfall extremes.

How to cite: Chen, M., Peleg, N., and Fatichi, S.: Quantifying Future Shifts in Intensity–Duration–Frequency (IDF) in Singapore: A comparison of methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14931, https://doi.org/10.5194/egusphere-egu25-14931, 2025.

Climate change is an essential part of sustainable development challenges in developing countries. Climate change represents one of the greatest environmental, social, and economic threats facing the world today. Accurate meteorological and hydrological projections are vital for effective climate adaptation and resource management, particularly under changing climate scenarios. However, the coarse spatial resolution of General Circulation Models (GCMs) limits their applicability for localized impact assessments. This study proposes a deep learning-based super-resolution approach combined with an advanced hydrological model to downscale and enhance the spatial resolution of three GCM datasets—GFDL-CM4, GISS-E2-1-G, and IPSL-CM6A-LR—to approximately 0.01°. The performance of the method is evaluated based on mean square error (RMSE), mean absolute error (MAE), Peak signal-to-noise ratio (PSNR), and Pearson correlation coefficient (R). This study hypothesizes to have more precise and accurate meteorological and hydrological predictions and projections under this framework. The model is conducted on historical climate data and compared with high-resolution observational datasets, showcasing its ability to capture fine-scale climatic and hydrological variability. This approach bridges the resolution gap in climate projections and provides a robust framework for better-informed decision-making in climate change adaptation and mitigation strategies.

Funding

This research was supported by Disaster-Safety Platform Technology Development Program of the National Research Foundation of Korea (NRF) funded by the Ministry of Science and ICT. (No. 2022M3D7A1090338).

How to cite: Huong, O. S. and Lee, G.: Improving Climate Change  Data through Deep Learning Super-Resolution Downscaling of GCMs for Precise Hydrological Projections, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15576, https://doi.org/10.5194/egusphere-egu25-15576, 2025.

EGU25-15818 | ECS | Orals | HS7.2

Hourly Precipitation Biases and Clausius-Clapeyron Scaling in Convection-Resolving and Convection-Parameterizing Regional Climate Models 

Alzbeta Medvedova, Isabella Kohlhauser, Douglas Maraun, Mathias W. Rotach, and Nikolina Ban

Regional climate models (RCMs) are crucial tools for understanding and predicting climate change and its impacts, such as precipitation extremes. We investigate the characteristics of hourly precipitation and the associated extremes in RCM ensembles with two resolutions: km-scale (the CORDEX-FPS Convection ensemble with ~3 km grid spacing, where deep convection is represented explicitly), and coarser-scale (~12 km grid spacing, with parameterized convection). The km-scale ensemble is downscaled from the coarser one, and both cover three time periods: evaluation, historical, and end-of-the-century period under the RCP8.5 warming scenario (2000-2009, 1996-2005, and 2090-2099, respectively). Evaluating the model ensembles against data from 179 weather stations in Austria, we study how the intensity, duration, and the time of onset of precipitation depend on mean daily temperature. We then examine how these characteristics change under warming conditions.

It is well established that over the Alps the coarser RCMs produce too much light and persistent precipitation which is triggered too early in the day. We find that these shortcomings in models with parameterized convection become more pronounced with rising temperatures. We show that the km-scale ensemble closely matches observations and greatly outperforms the coarser ensemble in capturing the investigated hourly precipitation characteristics, especially at higher temperatures and on days with heavy rainfall. As high temperatures are expected to become more common in future climates, our results imply that coarser RCMs suffer from more severe biases in hourly precipitation in the future than under present climate conditions, especially for short-duration extremes. 

In this light, we also assess the ability of both km-scale and coarser RCM ensembles to capture the Clausius-Clapeyron scaling of extreme precipitation with temperature, and discuss how model deficiencies in the coarser ensemble affect this relationship.

In summary, our findings highlight the importance of km-scale RCMs for accurate simulations of hourly precipitation and its extremes, particularly in the warming climate.

How to cite: Medvedova, A., Kohlhauser, I., Maraun, D., Rotach, M. W., and Ban, N.: Hourly Precipitation Biases and Clausius-Clapeyron Scaling in Convection-Resolving and Convection-Parameterizing Regional Climate Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15818, https://doi.org/10.5194/egusphere-egu25-15818, 2025.

EGU25-15936 | Posters on site | HS7.2

A Framework for Convection-Permitting Climate Downscaling over Southern Italy 

Giuseppe Mendicino, Luca Furnari, Elnaz Hatami Bahman Beygloo, Thomas Rummler, Harald Kunstmann, and Alfonso Senatore

Projecting climate change impact in southern Italy is particularly challenging because this region is located in the center of the Mediterranean basin, which is a recognized climate change hotspot, and is characterized by steep and complex orography requiring analysis at high spatial resolution. Therefore, climate models at the convection-permitting scale considerably improve the ability to simulate water cycle trends in that region, especially severe events.

This note introduces the modeling framework on which climate simulations are being carried out for southern Italy using CMIP6 projections and presents the first results related to the comparison of the historical simulation with observational datasets. A preliminary analysis revealed that the best CMIP6 global climate model (GCM) for reproducing the interannual cycle of precipitation and temperature over the study area is the High-Resolution MPI-ESM-1-2 model (1°x1° as horizontal resolution). Such a GCM was chosen to provide 6-hour boundary conditions for dynamic downscaling with the WRF (Weather Research and Forecasting) limited-area model with two domains one-way nested: the external one D01, with a horizontal resolution of about 20km, covering the entire Mediterranean area (209x214 grid points), and the internal one D02, with a horizontal resolution of about 4km, centered on southern Italy (285x265 grid points). The historical simulation extends from 1995 to 2014. The future simulations cover the period 2025 to 2045. The first future simulation employs the SSP 5-8.5 scenario.

Total precipitation and near-surface air temperature resulting from the historical simulation are compared with both observational datasets (namely, the spatially distributed products BigBang, SCIA, E-OBS, and validated weather station time series) and reliable downscaled reanalyses (e.g., ERA5-Land, MERIDA, MERIDA HRES, SPHERA, CERRA, VHREA_IT), which are increasingly available for the Italian peninsula. The results highlight that the evaluation of the performance of the historical simulation is partially affected by the selection of the reference dataset.

 

 

Acknowledgments: This study was funded by the Next Generation EU - Italian NRRP, Mission 4, Component 2, Investment 1.3, project WaterWISE - Water Management Strategies and Climate Change Adaptation in Southern Italy, n. PE00000005, CUP D43C22003030002; and by the Next Generation EU - Italian NRRP, Mission 4 ‘Education and Research’ - Component C2, Investment 1.1, Research Project of National Interest (PRIN 2022 PNRR) ­- An integrated modeling approach for mitigating climate CHANge effects through enhanCEd weathering in Southern Italy (CHANCES, CUP H53D23011260001), Italian Ministry of University and Research.

How to cite: Mendicino, G., Furnari, L., Hatami Bahman Beygloo, E., Rummler, T., Kunstmann, H., and Senatore, A.: A Framework for Convection-Permitting Climate Downscaling over Southern Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15936, https://doi.org/10.5194/egusphere-egu25-15936, 2025.

Precipitation time series are used as input for hydrological modeling. As the main driver of the hydrological cycle, they directly influence soil moisture, runoff, river flows, and groundwater recharge. High-resolution precipitation data is required to obtain accurate hydrological models. In addition, data should be available from different locations to reflect spatial dependencies in these models. As precipitation is measured only at selected locations, the simulated series can be used for design purposes.

In recent years, various models have been developed based on the Fourier Transform because of its ability to preserve desirable statistical properties. The concept is to transform the time series from the time domain to the frequency domain and calculate the two main components of the transformed series: the power spectrum (the square of the absolute values of the Fourier frequencies) and the phase spectrum (phase angle of the frequencies). The main idea behind all the Fourier-based models is to preserve the power spectrum because it relates to the autocorrelation function and overall structure.

This study compares the most common Fourier-based time series generators using different measures. As most spectral methods are iterative, this can be challenging for the precipitation time series, especially for the hourly resolution. In this regard, a non-iterative method is introduced. This method takes advantage of the Wiener–Khinchin theorem for the transformation between the autocorrelation function and the power spectrum. Another method, the Phase Annealing method, is introduced for precipitation time series generation and keeping the spatial and temporal properties. The results have been compared for the developed models and the most common Fourier-based methods.

How to cite: Mehrvand, M. and Bárdossy, A.: Comparative study of spectral methods for precipitation time series generators based on the conserving observed spatial and temporal properties, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16085, https://doi.org/10.5194/egusphere-egu25-16085, 2025.

EGU25-17581 | ECS | Posters on site | HS7.2

Daily precipitation dataset (1991-2021) at 1 km resolution over the Po river basin area using Kriging 

Sohaib Baig, Gaia Roatti, Marco Brian, Francesco Tornatore, Giuseppe Formetta, and Riccardo Rigon

The Po river basin, in the north of Italy, is the lifeline of the economic and ecology of the North of Italy. The 661 km long river covers an area of 71327 km2 and replenishes the water demands of agriculture, industry and domestic consumers. The topography is diverse  with alps mountains in the north and fertile plains in the south. The annual precipitation is 1200 mm which varies between ~2000 mm in the Alps to ~700 mm in the downstream. This study presents the estimates the precipitation on daily resolution over a grid of 1 km across the Po river basin for the period from 1991 to 2021, thus providing a consistent datasets for analyses of the recent climatology of the area. Total 1511 number of observed precipitation stations were included in the study along with topographic information. The statistical technique of kriging was employed to produce the grid data cube. The workflow of the study is summarized in the following steps:

  • obtain the meteorological data from the data providers
  • estimate the empirical semivariogram
  • fit theoretical models to the empirical semivariogram and analyses of the statistical correlation
  • use the theoretical model for solving the kriging system
  • produce continuous surface maps or time series of the quantity desired in any gridded point of the domain
  • calculate estimation errors.

For the estimation of errors Leave-one-out (LOO) is adopted which consists of removing a single station at a time and performing the interpolation for the location of the removed point by using the remaining stations. The approach is repeated until every station has been, in turn, removed and estimates are calculated for each station.

The results have shown that the average precipitation in the basin is 1131 mm with significant spatial patterns, some of which are reported for example. The northern subbasins have shown annual precipitation up to 2500 mm while the downstream planes receives up to 550 mm. The results show clear spatial and temporal patterns across the basin which  are reported in the study.

How to cite: Baig, S., Roatti, G., Brian, M., Tornatore, F., Formetta, G., and Rigon, R.: Daily precipitation dataset (1991-2021) at 1 km resolution over the Po river basin area using Kriging, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17581, https://doi.org/10.5194/egusphere-egu25-17581, 2025.

EGU25-19416 | ECS | Orals | HS7.2

Enhancing Extreme Rainfall Nowcasting with Weighted Loss Functions in Deep Learning Models 

Hyojeong Choi, Yongchan Kim, and Dongkyun Kim

With the increasing frequency and intensity of extreme rainfall events, the importance of nowcasting to minimize damage from disasters such as flash floods is becoming ever more prominent. However, most nowcasting models use loss functions aimed at minimizing the average prediction error. As a result, they tend to underestimate extreme rainfall—which has relatively low occurrence frequency but significant impact. In this study, we applied various types of weighted loss functions to a ConvLSTM-based nowcasting model to more accurately predict extreme rainfall. In particular, we varied parameters within these weighted loss functions and conducted sensitivity analyses to identify the optimal weighting strategies. We also categorized extreme rainfall types and evaluated the models’ predictive performance with weighted loss functions, thereby examining both the accuracy and stability of the model’s forecasts under extreme conditions from multiple perspectives. The results showed that the model employing a weighted loss function achieved significantly improved accuracy in predicting extreme rainfall, compared to an unweighted model. Furthermore, depending on the type of weighted loss function and parameter settings, the model demonstrated notably strong performance for specific types of extreme rainfall. This finding suggests that, in a rainfall environment characterized by high variability, dynamically selecting weighted loss functions according to forecasting objectives and conditions can enhance both the efficiency and reliability of extreme rainfall prediction. The approach presented in this study can be applied to flood forecasting and is anticipated to contribute to the advancement of deep learning–based disaster response systems, reducing the potential damage caused by natural disasters.

 

Acknowledgements

This work was supported by Korea Environment Industry & Technology Institute(KEITI) through R&D Program for Innovative Flood Protection Technologies against Climate Crisis Program(or Project), funded by Korea Ministry of Environment(MOE)(RS-2023-00218873).

How to cite: Choi, H., Kim, Y., and Kim, D.: Enhancing Extreme Rainfall Nowcasting with Weighted Loss Functions in Deep Learning Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19416, https://doi.org/10.5194/egusphere-egu25-19416, 2025.

EGU25-19913 | Orals | HS7.2

Postprocessing of rainfall forecasts over East Africa 

Fenwick Cooper, Shruti Nath, Masilin Gudoshava, Nishadh Kalladath, Ahmed Amdihun, Jason Kinyua, Hannah Kimani, David Koros, Zacharia Mwai, Christine Maswi, Asaminew Teshome, Samrawit Abebe, Isaac Obai, Jesse Mason, Florian Pappenberger, Matthew Chantry, Antje Weisheimer, and Tim Palmer

We test methods of postprocessing rainfall forecasts out to 7 days over East Africa.

Using the physical forecast models, IFS from ECMWF and GFS from NCEP, we apply several combinations of post-processing techniques to empirically correct the predicted rainfall towards IMERG blended satellite rainfall data. The techniques we apply include a generative adversarial neural network (GAN) model (Harris et al. 2022), isotonic distributional regression (EasyUQ, Walz et al. 2024), EMOS (Gneiting et al. 2005), linear regression, and the kernel density estimate. Other approaches are also considered, however for the purposes of practical operational forecasts, we mainly focus on computationally cheap methods. Because we are comparing against IMERG, our results compare favourably against fully empirical models, such as FuXi and Graphcast, that have been trained to predict ERA5.

Being computationally cheap, in an operational forecast cycle on a standard desktop computer, the GAN model can produce spatially correlated 1000 member ensembles from the input forecast data. from which we can display the distribution using a histogram. The other techniques also cheaply produce rainfall distributions. We compare the quality of these distributions using the CRPS, variogram score and reliability diagrams. Biases in the raw rainfall forecasts are most notably reduced over the large lakes, for example Lake Victoria, over mountains, Indian ocean, and other places of high rainfall. We find it difficult to reduce biases in dry regions and over the Congo rainforest.

Different empirical modelling methods are optimal for different physical phenomena, and there is no theory for the most accurate model without physical insight. We also observe that it is often possible to improve each of the models with various tweaks. Each of the tested approaches might improve in the future, and the question we are trying to answer is “what is the best practical model available today?”

How to cite: Cooper, F., Nath, S., Gudoshava, M., Kalladath, N., Amdihun, A., Kinyua, J., Kimani, H., Koros, D., Mwai, Z., Maswi, C., Teshome, A., Abebe, S., Obai, I., Mason, J., Pappenberger, F., Chantry, M., Weisheimer, A., and Palmer, T.: Postprocessing of rainfall forecasts over East Africa, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19913, https://doi.org/10.5194/egusphere-egu25-19913, 2025.

NP3 – Scales, Scaling and Nonlinear Variability

EGU25-735 | ECS | Posters on site | NP3.1

Decoding Typhoon Wind Patterns: Variational Retrieval and Multifractal Insights 

Jisun Lee, Seong-Jun Hwang, and Dong-In Lee

Typhoon wind dynamics are inherently nonlinear, exhibiting complex interactions between large-scale trajectory shifts and small-scale variability. This study employs variational retrieval techniques and multifractal analysis to investigate altitude-specific wind field patterns and their connections to trajectory and intensity changes. Using radar observations and numerical model data, high-resolution 3D wind fields were constructed to explore the structural and statistical characteristics of wind components (U, V) across different altitudes and typhoon trajectories.

Our analysis focuses on two distinct trajectory types: northward-moving typhoons (e.g., Nakri, Lingling, Bavi) and northeastward-moving typhoons (e.g., Chaba, Kong-Rey). Results indicate that northward trajectories exhibit crescent-shaped wind patterns dominated by northerly wind components, while northeastward trajectories show circular wind structures. Notably, multifractal analysis revealed abrupt decreases in the multifractal parameter α for northerly winds at 1–2 km altitude during trajectory transitions, suggesting nonlinear structural reorganization within the typhoon system. For example, during Typhoon Chaba (2016) and Typhoon Kong-Rey (2018), α values for northerly winds dropped sharply by 1.5–2.2 units, coinciding with significant directional shifts and rapid changes in typhoon directions.

In addition to wind field analysis, we quantified variability in rainfall fields using radar reflectivity and rainfall intensity data. Northeastward-moving typhoons demonstrated broader and more intense rainfall bands, with higher vertical reflectivity profiles up to 8 km altitude, compared to the narrower and more localized patterns observed in northward-moving cases. This suggests a strong coupling between wind field variability and rainfall distribution, driven by nonlinear interactions.

By integrating multifractal techniques with variational retrieval methods, this study bridges small-scale turbulence with large-scale trajectory dynamics, offering new insights into the inherent complexity of typhoon systems. These findings contribute to the development of advanced prediction systems, enabling more accurate trajectory and intensity forecasts. Such approaches could significantly mitigate the impacts of typhoons on the Korean Peninsula and beyond.

 

This work was supported by the National Research Foundation of Korea(NRF) grant funded by the Korea government(MSIT) (No.RS-2024-00460019)

How to cite: Lee, J., Hwang, S.-J., and Lee, D.-I.: Decoding Typhoon Wind Patterns: Variational Retrieval and Multifractal Insights, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-735, https://doi.org/10.5194/egusphere-egu25-735, 2025.

EGU25-1093 | ECS | Orals | NP3.1

Multifractal correlation of rainfall extremes and temperature 

Yann Torres Guimarães and Auguste Gires

Multifractal processes describe complex systems characterized by variability that spans across multiple scales and intensities, governed by scale-invariant distributions of extreme values. Universal Multifractals (UM) provide a robust framework for modelling and understanding the inherent extreme variability and scaling properties of various geophysical phenomena. It is a parsimonious framework that relies on only 3 parameters with physical interpretation, C1 the mean intermittency, α the multifractality index and H the non-conservation parameter.

 

Rainfall, inherently variable across spatial and temporal domains, has been widely studied in the framework of UM, with techniques like Trace Moment (TM) and Double Trace Moment (DTM) applied to characterize its scaling properties. Based on this framework, this study aims to assess the correlation between rainfall scaling features and extremes, and temperature ones, relying on multifractal analysis such as DTM and TM. High resolution simultaneously collected rainfall data from disdrometers and temperature data from meteorological stations is used. Data was collected during various measurement campaigns operated by the TARANIS observatory of HM&Co laboratory of Enpc (https://hmco.enpc.fr/portfolio-archive/taranis-observatory/). Data collected both in an urban area and on a meteorological mast located on a wind farm is used. For the disdrometer data, it was collected with 30 seconds time steps, As for the temperature, the meteorological station measures the temperature at 1Hz, so to match their time series it was necessary to take averages of the temperature data at each 30s.

 

Initially, the study explores the correlation between the primary multifractal parameters (C1, α, H) of rainfall and the average temperature at the rainfall event scale. Subsequently, a comparative analysis was conducted between these rainfall parameters and their counterparts derived from temperature fluctuations. This two-step approach aimed to uncover not only direct correlations between rainfall and temperature but also the extent to which the multifractal properties of rainfall mirror those observed in temperature dynamics. In a second part of the study, similar analysis on longer periods of typically one month are used to complement event based analysis by accounting for dry periods.

 

Authors acknowledge the ANR PRCI Ra2DW project supported by the French National Research Agency – ANR-23-CE01-0019-01 for partial financial support.

How to cite: Torres Guimarães, Y. and Gires, A.: Multifractal correlation of rainfall extremes and temperature, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1093, https://doi.org/10.5194/egusphere-egu25-1093, 2025.

EGU25-4129 | Posters on site | NP3.1

Multiscale Statistical Distribution of Porous Media Transport Behaviour: A Fractal Geometry Approach 

Wei Wei, Paul Glover, and Piroska Lorinczi

The transport properties of porous media exhibit complex multiscale behaviours, which are governed by nonlinear interaction of structural heterogeneity, and which present significant challenges for theoretical understanding and practical modelling. To address this complexity, we propose a fractal-based framework to quantitatively link structural parameters with transport behaviours, focusing specifically on electrical current flow in porous media. Our approach develops a tortuosity model based on self-similarity principles in order to describe the geometric structure, and to assess the transport properties, such as permeability and electrical conductivity.

At the single-capillary level, key microstructural properties, such as pore geometry and connectivity, and transport properties, including permeability and electrical conductivity, can be quantified using metrics such as fractal dimension, tube number, and characteristic length. These parameters capture both structural complexity and scaling behaviour. Taking electrical conductivity as an example, a two-dimensional porous medium with a grid resolution of 16,384 × 16,384 is generated using the Quartet Structure Generation Set (QSGS) method and partitioned into smaller scales (e.g., 1024, 512, 256, and 128) to explore multiscale behaviour and scaling effects. Finite difference methods are employed to calculate the electrical field distributions and derive the effective electrical conductivity. These results are then mapped to the parameters of the self-similar tortuosity model, providing insights into its ability to capture the complex relationships between structure and transport properties.

Statistical analysis reveals that the measured fractal dimensions follow a Weibull distribution across scales, characterised by its distinctive shape and scale parameters. By contrast, characteristic length and tube number values exhibit scale-dependent variations that influence their respective distribution patterns. Tube number conforms to a lognormal distribution, reflecting its intrinsic variability. These findings enable the development of more accurate and computationally efficient multiscale models, with potential applications in areas such as fluid flow, heat transfer, and the design of advanced porous materials.

How to cite: Wei, W., Glover, P., and Lorinczi, P.: Multiscale Statistical Distribution of Porous Media Transport Behaviour: A Fractal Geometry Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4129, https://doi.org/10.5194/egusphere-egu25-4129, 2025.

EGU25-8573 | ECS | Orals | NP3.1

What guides regime transitions in ecohydrological systems? 

Daniel F. T. Hagan, Benjamin L. Ruddell, Hsin Hsu, Yikui Zhang, and Diego G. Miralles

Changes in ecohydrological systems are driven by emergent patterns of organization that arise through internal differentiation, reflected in the variability of ecosystem components and shifts in the strengths of positive and negative feedbacks. This phenomenon, known as self-organization, allows ecosystems to transition between self-organized states in response to external perturbations, leading to new dynamic regimes. The resulting overall emergent properties represent a balance between the loss of stability and shifts toward equilibrium within ecosystems. However, it remains unclear whether ecosystem self-organization is guided by a convergence of states and feedbacks toward an optimal state and, if so, what such an optimal state might look like.

Using information-theoretic approaches, we characterize ecosystem variability and feedbacks as entropy changes based on observations. To do so, we concentrate on eddy-covariance measurements from global FLUXNET stations. Our findings reveal potential optimal states toward which ecosystems tend to transition and identify the conditions that govern these transitions, shaping the evolutionary trajectories of ecosystems. These results also provide a framework for assessing ecosystem resilience to major perturbations, such as droughts and heatwaves, and emphasize the critical role of hydrological variability in improving predictions of ecosystem changes and extreme events that pose risks to water and food security.

How to cite: Hagan, D. F. T., Ruddell, B. L., Hsu, H., Zhang, Y., and Miralles, D. G.: What guides regime transitions in ecohydrological systems?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8573, https://doi.org/10.5194/egusphere-egu25-8573, 2025.

EGU25-11882 | ECS | Orals | NP3.1

From Crisis to Adaptation: The Resilience of Critical Infrastructure in Recent Flood Events 

Sagnika Chakraborty, Nour Eddin El Faouzi, and Angelo Furno

As climate change accelerates, the frequency and intensity of flood events are rising, creating significant challenges for critical infrastructure systems worldwide. Transportation, energy, and communication networks are particularly vulnerable, and their resilience to such disasters
is crucial for minimizing long-term impacts. This study examines five recent flood events—Germany (2021), Belgium (2021), Sydney (2022), Auckland (2023), and Italy (2023)—to explore the effects of these floods on critical infrastructure and identify best practices for enhancing resilience. The research focuses on answering the central question:
How do recent flood events impact critical infrastructure, and what best practices can be identified for improving resilience?


Due to the recent nature of these floods, data collection was a pivotal aspect of the study, with information sourced from public news reports, research journals, government reports, and interviews. A Multi-Criteria Decision Making (MCDM) method- the Vikor, was employed to rank hazards, vulnerabilities, and the resilience of critical infrastructure in each case study. This approach provided a systematic evaluation of shared vulnerabilities and region-specific
differences in disaster response and infrastructure resilience.


The findings highlight the importance of multi-stakeholder collaboration, early warning systems, and adaptive infrastructure solutions in mitigating flood impacts. Best practices were identified across all phases of disaster management—pre-disaster preparedness, immediate emergency response, and long-term recovery. These practices emphasize the need for innovative infrastructure adaptations, community engagement, and coordinated
governance to build more resilient systems.


This research offers valuable insights for policymakers, urban planners, and disaster management professionals. By analyzing these five flood events, the study provides transferable lessons on how to enhance infrastructure resilience and integrate adaptive strategies into policy frameworks. Ultimately, this research contributes to the broader global discourse on climate adaptation and disaster risk reduction, aiming to strengthen preparedness
for future flood events.


Keywords: Flood resilience, critical infrastructure, case study analysis, MCDM, disaster management, data collection, best practices

How to cite: Chakraborty, S., El Faouzi, N. E., and Furno, A.: From Crisis to Adaptation: The Resilience of Critical Infrastructure in Recent Flood Events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11882, https://doi.org/10.5194/egusphere-egu25-11882, 2025.

EGU25-12865 | ECS | Orals | NP3.1

An investigation on the impact of intermittency on wind Lidar profiler data utilizing a Universal Multifractal framework  

Sonali Maurya, Auguste Gires, Ioulia Tchiguirinskaia, Daniel Schertzer, and Maxime Thiébaut

The intermittent nature of turbulence introduces significant variability and extreme events, which profoundly complicates efforts to accurately measure, model, and predict its behavior. In the context of the atmospheric boundary layer, this intermittent turbulence can lead to localized bursts of wind shear, which poses risks to wind energy operations. These fluctuations directly impact the operational efficiency and structural integrity of wind turbines. Specifically, turbulence influences fatigue loads on the turbines and is essential for accurately modeling wake effects that occur within wind farms, which can affect the performance of adjacent turbines and forecasting energy production. Research suggests that a multifractal framework characterized by complex patterns across various scales enables one to properly model the intermittency of turbulence. To investigate this phenomenon, the present study analyzes wind data collected using a state-of-the-art lidar (Light Detection and Ranging) system profiler. This profiler was deployed on an offshore measurement mast situated near an offshore wind farm located 13 kilometers off the coast of Fécamp, France. Employing a universal multifractal (UM) framework, this study seeks to simulate and analyze the extreme variability inherent in the collected data. In the first step, The UM framework will be used to quantify the effects of intermittency on standard metrics such as turbulence intensity (TI) and spectral slopes, also accounting for the resolution at which they are computed and the frequency of data. Empirical estimates of TI and spectral slope in homogeneous turbulence often deviate from theoretical scaling, which can be theoretically and empirically quantified. In the second step, the results of the UM analysis of the measured time series will be discussed. Additionally, this study will delve into the instrumental biases introduced by the lidar instrument used in the measurement of turbulence. These biases can significantly impact the accuracy of data interpretation and reliability of results, making it essential to explore and address them thoroughly. This research not only addresses the theoretical aspects of turbulence but also has practical implications for optimizing wind energy operations in the face of unpredictable environmental conditions. Finally, the authors would like to acknowledge the partial financial support of the French Government, managed by the Agence Nationale de la Recherche under the Investissements d’Avenir program, with the reference ANR-10-IEED-0006-34. This work was carried out in the framework of the NEMO project.

How to cite: Maurya, S., Gires, A., Tchiguirinskaia, I., Schertzer, D., and Thiébaut, M.: An investigation on the impact of intermittency on wind Lidar profiler data utilizing a Universal Multifractal framework , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12865, https://doi.org/10.5194/egusphere-egu25-12865, 2025.

Extreme events have a significant impact on nature, industry, agriculture, and society as a whole. From life-threatening heat waves and spring frosts that devastate crops in orchards and vineyards to other extremes such as epileptic seizures or financial market crashes, these phenomena remain a focus of intense scientific investigation.

The identification of causal relationships, specifically distinguishing cause from effect, is a rapidly advancing area of scientific research. Experts from various disciplines, including mathematics, physics, computer science, and others, are developing computational methods and algorithms to uncover causal links from experimental data.

Despite growing interest in these scientific fields, surprisingly few research teams integrate the study of causality with the analysis of extreme phenomena. Building on the information-theoretic generalization of Granger causality, Paluš et al. (2024) propose Rényi information transfer as a method for determining which of two or more potential causal variables gives rise to extreme values in an effect variable. Their study identifies the Siberian High as a key driver of increased probabilities of cold extremes in winter and spring surface air temperatures in Europe, while the North Atlantic Oscillation and blocking events are shown to induce shifts in the entire temperature probability distribution.

In this contribution we will employ Rényi information transfer to investigate the underlying causes of heat waves or warm extremes in summer surface air temperature in Europe. We will highlight the role of blocking events and examine the contribution of other relevant circulation phenomena, accounting for varying spatial and temporal scales as well as non-Gaussian probability distributions.

 

This research was supported by the Johannes Amos Comenius Programme (P JAC), project No. CZ.02.01.01/00/22_008/0004605, Natural and anthropogenic georisks, and by the Czech Academy of Sciences, Praemium Academiae awarded to M. Paluš.

 

Paluš, M., Chvosteková, M., & Manshour, P. (2024). Causes of extreme events revealed by Rényi information transfer. Science Advances, 10(30), eadn1721.

How to cite: Paluš, M.: Behind extreme variability: Unveiling causes using information theory beyond Shannon, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14307, https://doi.org/10.5194/egusphere-egu25-14307, 2025.

EGU25-14433 | ECS | Orals | NP3.1

One day in the life of clouds  

Paulina Patiño and Klaudia Oleschko

In 1870, Prof. Paey,  President of the Anthropological Society of Cuba, underlined that no one can ignore that studying clouds is one of the most practical needs of meteorology (1). More than 150 years later, the long-term stability of the Earth's atmosphere and climate (2) is recognized as sensitive to cloud dynamics (3), especially cloud thinning, relating it directly to climate change (4). The critical conclusion, documented in numerous studies (5), is that climate change is also a health crisis (6). The general panorama and the need to classify the clouds (7) to create a reliable Library for Machine Learning. Graph Geometric Algebra networks for graph representation learning (8) can become the decisive moment for cloud studies and modeling passing from classification to physics-informed Turing-like patterns recognition inside the diurnal variations of clouds and corresponding humidity profiles of the atmosphere. Multifractal and p-adic forecasting (9) of Big Data patterning is envisaged as the New Science of Complexity based on the physics of atmosphere, clouds, and climate (10, 11). Based on the physics-informed approach, we focus on original numbers systems and their multiscale pattering, fusing, and unifying Big Geo Data inside the probability-embedded medium, introducing the new methodology for Turning-type patterning quantifier of cloud system multiscale structure complexity extracted from physics-informed and statistics-informed raw data and images with moving space-temporal boundaries. Muuk'il Kaab (MIK) agile, bio-inspired (bees-type) software was designed and calibrated multiscale images from smartphones to high-precision photo cameras on clouds. This contribution shows more than ten years of testing as a new Metacomplexity Universal Quantitative Attribute (MCUQA) for complex pattern recognition, measurement, multiscale visualization, and skeletonization. Our research aims to optimize the fusion of multidimensional multiphysical raw data sets by the same nature-inspired bee-type software through data visualization, image analytics, virtualization, and the unification and forecasting of physics-informed measures with number theory.

Keywords: Big Data; data fusion; algebra of images; physics-informed 3D signals visualization; networks images geometrization; Complexity quantitative attributes; thermodynamic, multifractal, and p-adic forecasting.

References:

  • Poey, F. New classification of clouds. 1870, Nature 2:382-385.
  • Henderson-Sellers, A. Clouds and the long-term stability of the Earth's atmosphere and climate. Nature, 1979, 279260786-260788.
  • Bony, S., Stevens, B., Frierson; D.M.W., Jakob, Ch., Kageyama, M., Pincus, R., Shepherd; T.G., Sherwood, S.C., Siebesma, A.P., Sobel, A.,M. and Webb, M. Clouds, circulation and climate sensitivity. Nature Geoscience, 2015, 261- 268.
  • Sokol, A., Wall, C., & Hartmann, D.L. Greater climate sensitivity implied by anvil cloud thinning. Nature Geoscience, 2024, 17, 398-403.
  • What happens when climate and mental health crises collide? Nature, 628, 235.
  • Wong, C. Climate change is also the health crisis: These graphics explain Why. Nature, 624, 14-16.
  • Schirber, M. Nobel prize: Complexity, from atoms to atmospheres. 2021, Physics 14, 141.
  • Zhong, J., Cao, W. Graph Geometric Algebra networks for graph representation learning. 2025, Nature, Scientific Reports, 15, 170.
  • Dubrulle, B. 2022. Multifractality, Universality and Singularity in Turbulence. 2022. Fractal and Fractional, 6, 613.
  • Mason, B.J. Physics of clouds and precipitation. 1954. Nature, 20, 957-959.
  • Bracco, A., Brajard, J., Dijkstra, H.A., Hassanzadeh, P.,, Ch. 2025. Machine learning for the physics of climate. Nature Reviews Physics, 7, 6-20.

How to cite: Patiño, P. and Oleschko, K.: One day in the life of clouds , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14433, https://doi.org/10.5194/egusphere-egu25-14433, 2025.

Climate network (CN) analysis has demonstrated significant potential and is widely applied in climate research. However, revealing the underlying mechanisms behind the results obtained from CN analysis remains challenging. One possible reason for this difficulty lies in the method used to determine the links between nodes in the climate network. The commonly used Pearson correlation analysis may not be able to fully capture the complex dynamics of the climate system. In particular, the multi-scale interactions among multiple processes may induce scaling behaviors in the climate system, which further lead to long-term climate memory. The presence of such memory may influence CN analysis outcomes. In this work, we aim to identify the climate memory impacts on the CN analysis. Combining with the Fractional Integral Statistical Model (FISM), we proposed a new approach named as CN-FISM. The FISM model allows for the extraction of the climate memory component, enabling the modification of time series to preserve a specified length of memory. By conducting CN analysis on these adjusted series, one thus can quantify the impacts of climate memory. This approach has been successfully employed to a recent CN analysis on the Pacific Decadal Oscillation (PDO) phase change. Compared with the current Pearson correlation-based CN approach, the CN-FISM may enhance the interpretability of CN results.

How to cite: Yuan, N. and Wei, Z.: Identifying climate memory impacts on climate network analysis using fractional integral techniques, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15394, https://doi.org/10.5194/egusphere-egu25-15394, 2025.

EGU25-17717 | ECS | Orals | NP3.1

 Scaling relationships in hydrological quantities and pollutant loads across river basins 

Louise Schreyers and A. Jan Hendriks

Quantities such as discharge, flow velocity, water depth, and pollutant loads are essential for understanding pollutant emissions and for effective hydrological management, including flood control, water supply, and ecosystem preservation. Despite their critical importance and advances in data collection and modeling, the challenge of predicting these quantities in ungauged or poorly monitored basins persists. In the case of pollutants, this issue is complexified by the growing number of pollutants requiring evaluation. For example, within the EU, more than 100,000 chemical compounds require assessment.

Scaling relationships, which relate system characteristics to basin size metrics, offer a promising stepping stone to address this challenge. For instance, river discharge - one of the most fundamental hydrological metrics - has been shown to scale with basin size through power-law relationships. This scaling is also influenced by additional factors such as climatic conditions, land use, and geomorphology, underscoring the need for integrated approaches to characterize the scaling relationship. Similarly, pollutant loads are often expressed through models such as the Concentration-Discharge (C-Q) relationship, which links pollutant concentrations (C) to discharge rates (Q). While such models provide valuable insights, their applicability requires robust scaling principles to account for variability in pollutant sources, and transport mechanisms. 

In this contribution, we present our framework to derive scaling relationships for key quantities in the hydrological cycle and pollutant loads within river basins, focusing on their dependence on size-related indicators of river basins. Scaling principles of metrics such as discharge, flow velocity, water depth, and groundwater volume are derived using observational datasets, such as Global Runoff Data Center and SWOT river database. For pollutant loads and emissions, where monitoring is limited to a few key indicators, scaling principles offer promising avenues to predict emissions across diverse systems. By linking hydrological and pollutant-related variables through consistent scaling principles, we aim to provide a unified approach to understanding variability across river basins of different sizes. This work underscores the value of scaling relationships in bridging theoretical insights and practical applications, offering tools for improved management of water resources and pollutant impacts.

How to cite: Schreyers, L. and Hendriks, A. J.:  Scaling relationships in hydrological quantities and pollutant loads across river basins, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17717, https://doi.org/10.5194/egusphere-egu25-17717, 2025.

EGU25-20443 | Posters on site | NP3.1

Nonlinear dynamics and intermittency of the solar wind magnetic field fluctuations probed with surrogate data 

Eliza Teodorescu, Marius Echim, and Jay Johnson

We present a statistical approach to estimate the significance of the intermittency of solar wind magnetic field fluctuations. We analyze nine days of magnetic field data provided by Parker Solar Probe (PSP) at about 0.17 AU from the Sun during the probe’s first perihelion (Encounter 1). Intermittency is estimated based on flatness, the normalized fourth-order moment of the probability distribution functions. When we divide the signal in sub-intervals of 3 to 24 hours length, we find that flatness/intermittency varies from interval to interval. Sub-intervals showing very low levels of intermittency, with flatness values close to three at all scales, alternated with highly intermittent sub-intervals where flatness reaches values close to 60.

In order to understand the observed variability of the intermittency level, we applied a statistical test based on data surrogates (Theiler et al., 1992) tailored to identify nonlinear dynamics in a time series. The aim is to falsify a null hypothesis that is a-priori known to be invalid, i.e. the intermittency observed in PSP data results from a linear Gaussian-like physical process, with the nonlinearity being due to the observation function.

The surrogates are generated such that all nonlinear correlations contained in the dynamics of the signal are eliminated. We find that the flatness computed for the original signal is significantly different from that computed for the ensemble of surrogates, i.e. the null hypothesis is falsified. Thus, the flatness is indeed a descriptor of the intermittency resulting from the inherent nonlinear dynamics of the process captured by the magnetic field observations of the PSP. We also discuss how the non-stationarity of a time series affects the flatness computed for both the PSP data and the surrogates, precluding the null hypothesis is falsified.

Further, a multi-order simultaneous fit of the structure functions revealed a decrease in flatness at scales smaller than a few seconds: intermittency is reduced in this scale range. This behavior was mirrored by the spectral analysis, which was suggestive of an acceleration of the energy cascade at the high frequency end of the inertial regime.

How to cite: Teodorescu, E., Echim, M., and Johnson, J.: Nonlinear dynamics and intermittency of the solar wind magnetic field fluctuations probed with surrogate data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20443, https://doi.org/10.5194/egusphere-egu25-20443, 2025.

EGU25-20554 | Orals | NP3.1

Multifractal Phase Transitions for the “Transformative Shift” Towards a Shared Value Economy 

Ioulia Tchiguirinskaia, Guillaume Drouen, Yangzi Qiu, Pierre-Antoine Versini, Auguste Gires, and Daniel Schertzer

International projections indicate that extreme climatic events will become more frequent and intense, leading to significant disruptions in water cycle patterns. At the same time, water remains the only irreplaceable natural resource. As a result, human economies must be prepared to confront a range of socio-economic challenges stemming from changes in the water cycle. These issues cannot be resolved through incremental improvements to existing measures. Consequently, there is a growing call for "transformative change" — a comprehensive, system-wide restructuring at various scales, akin to what physicists describe as a non-equilibrium phase transition in a complex, nonlinear system — to tackle the interconnected and persistent challenges.

In recent years, there has been a growing global emphasis on funding research with greater "transformative impact." This often leads to a focus on the outcomes and content of transformative change, when the real focus should be on the underlying physics, as achieving transformative change depends fundamentally on the interactions of these underlying processes. The scientific challenge common to both socio-economic and hydrological systems lies in their pronounced spatio-temporal heterogeneity and variability within urban environments. This variability arises from the highly nonlinear interactions among the relevant variables, which produce extreme multiscale fluctuations and complex causal chains, beginning with the fact that responses are not proportional to the initial stimuli or forces.

Urban geosciences introduce additional complexity compared to traditional geosciences: their physical scales are much smaller, requiring not only higher-resolution observation technologies, which is already a significant challenge, but also involve much shorter interaction times. This shorter timescale is particularly crucial for prediction, as it limits the predictability of these systems. In this context, universal multifractals (multiplicative stochastic processes) likely provide the most effective framework for establishing a common foundation that supports more diverse and collectively potent approaches to transformative environmental change. Gaining a deeper understanding of multifractal phase transitions and their practical application, alongside alternative innovations, is key to fostering transformative change.

To promote such transitions, this presentation will focus on non-trivial symmetries to address much of the complexity outlined earlier. A key example is scale symmetries, which allow for the definition of scale-independent observables, in contrast to classical observables that are heavily dependent on scale. This scale dependence creates several challenges, starting with the fact that the models based on these observables are also scale-dependent. Scale-independent observables, often referred to as singularities, are significant because they capture the divergence of classical observables as resolution increases, or as we look at progressively smaller scales. The strength of this approach lies in its application to urban geosciences, specifically for: (i) defining environmental indicators for cities and their characteristics, (ii) monetizing the amenities provided by blue-green solutions in urban areas and contextualizing them socio-economically on a large scale, and (iii) developing a new form of multifractal evaluation for environmental balance - altogether enabling "transformative chift" towards the sheared value economy.

The authors sincerely acknowledge the partial financial support provided by the TIGA CfHf project (https://hmco.enpc.fr/portfolio-archive/tiga/).

How to cite: Tchiguirinskaia, I., Drouen, G., Qiu, Y., Versini, P.-A., Gires, A., and Schertzer, D.: Multifractal Phase Transitions for the “Transformative Shift” Towards a Shared Value Economy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20554, https://doi.org/10.5194/egusphere-egu25-20554, 2025.

EGU25-20565 | Posters on site | NP3.1

Combining Artificial Intelligence and Multifractals for Precipitation Nowcasting: the UM-GAN Example. 

Daniel Schertzer, Hai Zhou, and Ioulia Tchiguirinskaia

Intermittency is a defining characteristic of rainfall, yet it is largely overlooked in most IA nowcasting models. We emphasise its theoretical significance at various stages of the prediction process, from training to assessing its accuracy, including its dispersion relative to the intrinsic limits of predictability. 

Specifically, we develop a hybrid framework based on:

  • - The generative adversarial network (GAN), a recently developed technique for training IA models through an adversarial process;
  • Universal multifractals (UM), stochastic models of intermittency that are physically based on the cascade paradigm. They are universal in the sense that they are statistically attractive to other processes and depend only on three scale-independent parameters that are physically meaningful.

 In terms of physical relevance, we evaluate the nowcasting performance of the hybrid UM-GAN model and other baseline models (ConvLSTM, GAN) using continuous and categorical scores, as well as UM analysis in comparison to the observations. The results indicate that UM-GAN achieves the highest scores and accuracy, particularly demonstrating superior performance at lead times of 30 minutes and 60 minutes.

How to cite: Schertzer, D., Zhou, H., and Tchiguirinskaia, I.: Combining Artificial Intelligence and Multifractals for Precipitation Nowcasting: the UM-GAN Example., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20565, https://doi.org/10.5194/egusphere-egu25-20565, 2025.

EGU25-283 | ECS | Orals | OS1.9

Drivers of sensible heat flux in the Southern Ocean and their relationship to submesoscale fronts 

Johan Edholm, Hanna Rosenthal, Louise Biddle, Sarah Gille, Matthew Mazloff, Marcel du Plessis, and Sebastiaan Swart

Advances in uncrewed surface vehicles (USVs) enable expanded observations in the Southern Ocean, a region vital for global heat uptake yet critically undersampled. Using data from three USVs that sampled the Pacific sector of the Southern Ocean in both summer and winter, we evaluate processes and decorrelation scales driving sensible heat flux variability. High flux variability is linked to synoptic-scale southwesterly winds, with sensible heat flux decorrelation scales of 40–60 km and 6–10 hours, consistent across seasons and variables. Fine-scale (<1–10 km) oceanic processes, including fronts, filaments, and boundaries, further influence flux variability: Our datasets reveal over 8,000 temperature fronts ranging from <1 km to >20 km in width. While wind-related variability dominates sensible heat flux changes across the smallest fronts, the ocean’s role becomes increasingly significant with front width, reaching parity at ~4 km. However, due to their abundance, the total change of sensible heat flux over smaller (~1 km) fronts is an order of magnitude greater than that of larger (>4 km) fronts. These results highlight the role of fine-scale atmosphere-ocean interactions in driving heat flux variability in the Southern Ocean, offering valuable insights for enhancing flux estimates in this critical region.

How to cite: Edholm, J., Rosenthal, H., Biddle, L., Gille, S., Mazloff, M., du Plessis, M., and Swart, S.: Drivers of sensible heat flux in the Southern Ocean and their relationship to submesoscale fronts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-283, https://doi.org/10.5194/egusphere-egu25-283, 2025.

EGU25-1399 | Orals | OS1.9

 Dependence of dense filament frontogenesis in a hydrostatic model  

Yalin Fan and Zhitao Yu

 

 In this study, a hydrostatic model - the Navy Coastal Ocean Model (NCOM) is used to analyze the temporal evolution of a cold filament under moderate wind (along / cross filament) and surface cooling forcing conditions. The experimental framework adhered to the setup used in large eddy simulations by Sulllivan and McWilliams (2018). For each forcing scenario, the impact of horizontal resolutions is systematically explored through varies model resolutions of 100 m, 50 m, and 20 m; and the influence of horizontal mixing is investigated by adjusting the Smagorinsky constant within the Smagorinsky horizontal mixing scheme. The role of surface gravity waves is also assessed by conducting experiments both with and without surface wave forcing. 

The outcomes of our study revealed that while the hydrostatic model is able to predict the correct characteristics/physical appearance of filament frontogenesis, it fails to capture the precise dynamics of the phenomenon. Horizontal mixing parameterization in the model was found to have marginal effect on frontogenesis, and the frontal arrest is controlled by the model’s subgrid-scale artificial regularization procedure instead of horizontal shear instability. Consequently, higher resolution is corresponding to stronger frontogenesis in the model. Thus, whether the hydrostatic model can produce realistic magnitude of frontogenesis is purely dependent on the characteristic of the front/filament simulated and model resolution. Moreover, examination of the parameterized effect of surface gravity wave forcing through vertical mixing unveiled a limited impact on frontogenesis, suggesting that the parameterization falls short in representing the real physics of wave-front interaction. 

How to cite: Fan, Y. and Yu, Z.:  Dependence of dense filament frontogenesis in a hydrostatic model , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1399, https://doi.org/10.5194/egusphere-egu25-1399, 2025.

EGU25-2211 | Orals | OS1.9

ODYSEA: a satellite mission to advance knowledge of ocean dynamics and air-sea interaction 

Tong Lee, Sarah Gille, Fabrice Ardhuin, Mark Bourassa, Paul Chang, Sophie Cravatte, Gerald Dibarboure, Tom Farrar, Melanie Fewings, Fanny Girard-Ardhuin, Gregg Jacobs, Zorana Jelenak, Florent Lyard, Jackie May, Elisabeth Rémy, Lionel Renault, Ernesto Rodriguez, Clément Ubelmann, Bia Villas Bôas, and Alex Wineteer

Ocean-surface vector winds, currents, and their interaction play critical roles in shaping many aspects of the Earth’s environment (e.g., weather, climate, marine ecosystems, and ocean health), affecting human safety and wellbeing both on land and at sea. However, there are significant capability gaps in observing winds, currents, and their interaction. At present, global gridded products of surface currents have coarse (~150 km) feature resolutions and rely on theoretical assumptions that break down near the equator. Moreover, there is no satellite that provides simultaneous wind-current measurements that are important for studying wind-current coupling and its impact on weather and climate. The “Ocean DYnamics and Surface Exchange with the Atmosphere” (ODYSEA) satellite mission concept is designed to alleviate these capability gaps. ODYSEA, proposed to NASA’s Earth System Explorers program in mid-2023, aims to provide the first-ever global measurements of total surface currents and simultaneous winds with 5-km data postings and near-daily coverage of the global ocean. ODYSEA builds on NASA’s heritage of scatterometry and the success of the airborne Doppler scatterometer flown as part of the Sub-Mesoscale Ocean Dynamics Experiment (S-MODE), NASA’s Earth Venture Suborbital-3 (EVS-3) mission. ODYSEA also leverages strong domestic and international partnerships. Here we present ODYSEA’s objectives, anticipated capabilities, and expected contributions to advance the understanding of surface current dynamics and air-sea interaction.

 

How to cite: Lee, T., Gille, S., Ardhuin, F., Bourassa, M., Chang, P., Cravatte, S., Dibarboure, G., Farrar, T., Fewings, M., Girard-Ardhuin, F., Jacobs, G., Jelenak, Z., Lyard, F., May, J., Rémy, E., Renault, L., Rodriguez, E., Ubelmann, C., Villas Bôas, B., and Wineteer, A.: ODYSEA: a satellite mission to advance knowledge of ocean dynamics and air-sea interaction, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2211, https://doi.org/10.5194/egusphere-egu25-2211, 2025.

EGU25-3214 | Orals | OS1.9

Contribution of the air entrainment to the gas transfer processes in wave-breaking events 

Alessandro Iafrati, Sergio Pirozzoli, and Simone Di Giorgio

Gas exchange processes at the air-sea interface play a crucial role in regulating the climate and sustaining human and marine life. It is known that a large portion of anthropogenic carbon dioxide is absorbed by the ocean, which, in turn, releases nearly half of the oxygen we breathe through the photosynthesis of marine flora in the sunlit upper ocean layer. 

Despite its relevance, the processes governing the gas transfer across the ocean surface are not fully understood. Although there is evidence that the bubbles generated by the wave breaking enhances significantly the gas transfer rate, in particular for low-solubility species, the parameterization of their contribution is inaccurate.

To investigate the phenomenon, the gas transfer occurring at the free surface of progressive waves is simulated by using high-fidelity simulations. A multiphase flow solver is employed to model the gas flux across the air-water interface and the diffusion processes in the air and water domains, making available data with a level of detail unattainable in experiments. Waves of different initial steepness leading to regular wave patterns, mild spilling, and intense plunging breakers are examined and comparisons in terms of the gas flux across the interface and the gas concentration in the two fluids are established. 

It is shown that the amount of gas transferred from the air to the water domain increases remarkably when wave breaking occurs, particularly in the presence of bubble entrainment. The availability of such detailed information allows us to compute the gas transfer velocity. Critical in this respect is the availability of the air-water interface actual area, a quantity generally unavailable in experiments. The increase in the gas transfer velocity is higher than the increase in the interface area across which the exchange takes place, meaning that there is an additional effect related to the enhanced turbulence associated with the bubble entrainment and the subsequent fragmentation process. It is also observed that provided the actual air-water interface area is accounted for, the gas transfer velocity scales approximately as the one-fourth power of the dissipation rate of the energy content in water, consistently with previous theoretical predictions.

How to cite: Iafrati, A., Pirozzoli, S., and Di Giorgio, S.: Contribution of the air entrainment to the gas transfer processes in wave-breaking events, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3214, https://doi.org/10.5194/egusphere-egu25-3214, 2025.

EGU25-3897 | ECS | Posters on site | OS1.9

Different Trajectory Patterns of Ocean Surface Drifters Modulated by Near-inertial Oscillations 

Yuhang Zheng, Wei Wu, Minyang Wang, Yuhong Zhang, and Yan Du

Near-inertial oscillations (NIOs) are widely observed dynamic motions in the global ocean, with a frequency related to earth’s rotation. Using a particle trajectory model, we found the combined influence of mesoscale eddies and NIOs could produce distinctive flower-like trajectories, which are a special case of near-inertial trajectories and were observed by surface drifters released within an anticyclone eddy in the South China Sea in 2021. The energy budget indicates that wind and geostrophic eddy currents are crucial in generating near-inertial energy during the flower-like trajectories. Furthermore, the particle trajectory model revealed variations in periods and widths of the near-inertial trajectory with latitudes. The width of near-inertial trajectories can exceed 8km in the near-equatorial region and reach 3-6km in the mid-latitude region (20°-50°). The ratios of near-inertial velocity to background velocity, defined as NITSIs, lead to arc-shaped (0.5<NITSI<1.0), overlapping semi-circular (NITSI>1.0), and near-circular trajectories (NITSI>>1.0). Globally, approximately 1/3 of the drifters’ lifespan featured clear near-inertial trajectories, with a significant presence in most middle latitudes and the largest NITSI in the north Pacific westerly. These findings highlight the importance of NIOs and suggest their substantial impact on local surface matter distribution, trajectory prediction, and marine rescue operations.

How to cite: Zheng, Y., Wu, W., Wang, M., Zhang, Y., and Du, Y.: Different Trajectory Patterns of Ocean Surface Drifters Modulated by Near-inertial Oscillations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3897, https://doi.org/10.5194/egusphere-egu25-3897, 2025.

EGU25-5067 | ECS | Posters on site | OS1.9

Ocean-Atmosphere Coupling Processes during Typhoons in the East China Sea 

Bowen Du and Hui Wu

Typhoons, as intense ocean-atmosphere interaction events, exert profound impacts on coastal regions. The path and intensity of typhoons are predominantly governed by oceanic and atmospheric processes. While extensive research has been conducted in deep ocean regions, the mechanisms of ocean-atmosphere heat exchange during typhoon events remain inadequately understood in shallow shelf regions. It’s particular in the East China Sea, which is distinguished by its expansive continental shelf, shallow depths, overlapping surface and bottom mixed layers, and the influences of shelf circulation and the Yangtze River plume. In this region, tides are one of the key driving forces influencing ocean dynamics, however, they are rarely considered in ocean-atmosphere coupling studies. Basing on these, we have developed a high-resolution ocean-atmosphere coupled model for the coastal waters of China using the COAWST (Coupled-Ocean-Atmosphere-Wave-Sediment Transport) modeling system. This effort builds upon our research group's established high-resolution ocean model. Through simulations and validations of typhoon events, preliminary results demonstrate that ocean-atmosphere coupling significantly improves the prediction of typhoon tracks and intensities. This study will further analyze the dynamics of ocean-atmosphere heat flux exchanges during typhoons under the influence of shelf processes and examines their impacts on typhoon paths and intensities, with particular attention to the role of tides. These findings provide new insights into the dynamic processes induced by typhoons in coastal shelf regions and advance our understanding of their interactions with shallow ocean systems.

How to cite: Du, B. and Wu, H.: Ocean-Atmosphere Coupling Processes during Typhoons in the East China Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5067, https://doi.org/10.5194/egusphere-egu25-5067, 2025.

With the growth in computing power and the advancement in numerical algorithms, computational fluid dynamics (CFD) is playing an increasingly important role in the study of many fluid mechanics problems in geophysical sciences.  Built on highly accurate numerical schemes and utilizing high-performance computing, high-fidelity CFD is especially valuable for faithfully capturing the flow physics of turbulence in complex environments, such as water waves.  This talk will introduce some of our recent developments in numerical methods for nonlinear wave fields and turbulence in the wave environment.  The flow physics of wave-turbulence interaction will be illustrated, focusing on the turbulent boundary layers and multiphase flows at the wave surface.  Innovative theoretical analyses and modeling will be presented to reveal the underlying flow dynamics. 

How to cite: Shen, L.: Simulation-Based Study of Turbulent Flows in Wave Environment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5153, https://doi.org/10.5194/egusphere-egu25-5153, 2025.

EGU25-5418 | ECS | Posters on site | OS1.9

Impacts of Dust on Surface-Radiative Fluxes, and Sea Surface Temperatures in the Red Sea 

Sravanthi Nukapothula, Hari Prasad Dasari, Ravi Kumar Kunchala, Vassilis P. Papadopoulos, Ibrahim Hoteit, and Yasser Abualnaja

This study examines the impact of dust on surface and radiative fluxes, as well as sea surface temperature (SST), over the Red Sea during the dust season (March to August) from 1980 to 2024 using reanalysis and satellite datasets. We first identfied the extreme dust days (EDDs) across the Arabian Peninsula using MERRA-2 reanalysis data, employing the mean and two-sigma standardized deviation method. A total of 1,083 EDDs were detected during the study period, with 394, 103, and 39 days exclusively affecting the southern Red Sea, northern Red Sea, and the entire Red Sea, respectively.

We analysed the key variables, including dust aerosol optical depth, wind patterns, surface fluxes (latent and sensible heat), radiative fluxes (longwave and shortwave), and SST anomalies for the Red Sea and its sub-regions during EDDs. Positive anomalies in dust aerosol optical depth were observed over all three regions during EDDs, and further identified the dust transport pathways based on wind analyses. The results show significant radiative impacts, including increased longwave radiation (+16 W/m²) and reduced shortwave radiation (-30 W/m²) with suppressed latent heat flux (-50 W/m²) and sensible heat flux (-10 W/m²), indicating substantial ocean heat loss through surface evaporation during EDDs.

The SST anomalies also revealed a notable cooling across the Red Sea, with the northern region cooling up to -1.4°C, and the southern region exhibited milder cooling ranging between -0.3°C and +0.2°C. The average cooling across the entire Red Sea is approximately -0.8°C reflects the combined effects of stronger cooling in the northern and moderate cooling in the southern Red Sea region during EDDs. These findings highlight the critical role of dust in modulating surface energy budgets and SST variability in the Red Sea under three different EDD scenarios.

Key words: Arabian Peninsula, Extreme Dust Days, The Red Sea, Suraface-Radiative Fluxes, and Sea Surface Temperature.

How to cite: Nukapothula, S., Dasari, H. P., Kunchala, R. K., Papadopoulos, V. P., Hoteit, I., and Abualnaja, Y.: Impacts of Dust on Surface-Radiative Fluxes, and Sea Surface Temperatures in the Red Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5418, https://doi.org/10.5194/egusphere-egu25-5418, 2025.

EGU25-5512 | Posters on site | OS1.9

Development and evaluation of the probability density distribution for mixed layer depth over the global oceans 

Sergey Gulev, Vladimir Kukushkin, and Anne Marie Treguier

Development of theoretical probability density function (PDF) for MLD over the oceans is important, as such a function provides a novel avenue for diagnostics of the numerical experiments with ocean GCMs and for comparison of the model results with observational data such as Argo floats. We built a new PDF based upon the Censored Modified Fisher-Tippet distribution (CMFT PDF herein). CMFT PDF represents a 2.5 – parameter distribution with the shape and location parameters steering the PDF and a pre-defined minimum of sample. CMFT distribution provides explicit equations for the mean and variance and also allows for estimating extreme values of MLD corresponding to high percentiles. A newly developed CMFT PDF was applied to GLORYS12 reanalysis to diagnose the characteristics of MLD in terms of MLD statistics. For application we used 3-degree spatial averaging of GLORIS12 profiles to provide the results which can further analyzed and intercompared to different alternative MLD estimates. This provided quite a rich sample which was further used for computation of the PDF parameters and higher order percentiles over the global oceans. This analysis shows that characteristics of probability density distributions are quite different for different regions with e.g. Labrador Sea demonstrating much heavier tails compared to the Irminger Sea and the NAC. Extreme values of MLD for March can amount to more than 3000 meters in the Labrador Sea. This provides an effective diagnostic approach for intercomparison of different model experiments and also for validation of the model results against observational data, such as e.g. Argo buoys. We also provide the analysis of climate variability of MLD statistics derived from CMFT PDF demonstrating in particular different tendencies in the mean and extreme MLD values. Further we also discuss the links between the statistics of the ocean MLD with those of surface fluxes as well as atmospheric variability.

How to cite: Gulev, S., Kukushkin, V., and Treguier, A. M.: Development and evaluation of the probability density distribution for mixed layer depth over the global oceans, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5512, https://doi.org/10.5194/egusphere-egu25-5512, 2025.

Observations of Argo profiles and TAO/TRITON array confirm the significant seasonality of the barrier layer (BL) and temperature inversion (TI) in the northeastern tropical Pacific (NETP). Statistical result of the occurrence based on the Argo profiles reveals a bimodal variability of the BL, with two peaks in July and October. This bimodal seasonality of BL is attributed to the out-of-phase variations of the eastern Pacific fresh and warm pools. The fresh and warm pools both expand westward from May to July, when the Inter-Tropical Convergence Zone (ITCZ) becomes intense and broad. Heavy rainfall is the dominant contributor to the extension of the fresh and warm pools, leading to a high frequency of thick BL (40%). This frequent thick BL provides a precondition for its another development after August. The fresh pool is stable from August to November, while the warm pool contracts sharply. The cold tongue becomes active due to a prevailing trade wind and horizontal advection transports surface cold water to the northeastern warm pool. This cold advection deepens the isothermal layer and contributes to a frequent TI (30%) and thick BL (46%). The results suggest that the ITCZ rainfall and northward cold advection from equator dominate the upper layer stratification of NETP in summer and autumn, respectively 

How to cite: Chi, J.: The Impact of the Eastern Pacific Fresh and Warm Pools on the Bimodal Seasonality of Barrier Layers, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5569, https://doi.org/10.5194/egusphere-egu25-5569, 2025.

EGU25-5682 | ECS | Orals | OS1.9

Toward a better understanding of the effects of mesoscale air-sea interactions on the Antartic Circumpolar Current dynamics using coupled ocean-atmosphere models 

Anjdy Borg, Lionel Renault, Guillaume Lapeyre, Guillaume Morvan, Julien Jouanno, and Sallée Jean-Baptiste
Strong westerly winds blowing in the Southern Ocean enhance a unique oceanic dynamic composed of the world's strongest ocean current, the Antarctic Circumpolar Current (ACC), and a vertical circulation, the Overturning Circulation. Although these currents play a central role in shaping our climate, and despite numerous international observational and modeling programs, the processes controlling their strength and variability remain poorly understood, especially those related to fine-scale oceanic processes and their interactions with the atmosphere. To fill this gap, this study aims to understand both the direct and indirect effects of air-sea interactions on the dynamics of the ACC, including the large-scale, mesoscale (10-100 km), and eddy mean flow interactions (the inverse and direct energy cascade). We focus on two main air-sea interactions: the current feedback (CFB), which corresponds to the influence of surface ocean currents on the overlying atmosphere, and the thermal feedback (TFB), which is essentially the influence of ocean surface temperature and its gradients on heat and momentum fluxes. To achieve our goals, we developed a first set of coupled ocean (CROCO) - atmosphere (WRF) simulations of an idealized atmospheric storm track coupled to an idealized ACC with a spatial resolution up to 4 km for the ocean and 10 km for the atmosphere for a period of 75 years. We will present our first results, focusing in particular on the mean oceanic and atmospheric dynamics and the exchange of kinetic and potential energy between the ocean and the atmosphere.

How to cite: Borg, A., Renault, L., Lapeyre, G., Morvan, G., Jouanno, J., and Jean-Baptiste, S.: Toward a better understanding of the effects of mesoscale air-sea interactions on the Antartic Circumpolar Current dynamics using coupled ocean-atmosphere models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5682, https://doi.org/10.5194/egusphere-egu25-5682, 2025.

Mesoscale eddies are ubiquitous features of the global ocean circulation. Tradiontally, anticyclonic eddies are thought to be associated with positive temperature anomalies while cyclonic eddies are associated with negative temperature anomalies. However, our recent study found that about one-fifth of the eddies identified from altimeter data are surface cold-core anticyclonic eddies (CAEs) and warm-core cyclonic eddies (WCEs). Idealized numerical model experiments highlight the role of relative wind-stress-induced Ekman pumping, surface mixed layer depth, and vertical entrainment in the formation and seasonal cycle of these unconventional eddies. The abundance of CAEs and WCEs in the global ocean calls for further research on this topic.

How to cite: Zhai, X.: Cold anticyclonic eddies and warm cyclonic eddies in the ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5720, https://doi.org/10.5194/egusphere-egu25-5720, 2025.

EGU25-5858 | ECS | Orals | OS1.9

Intensification of Pacific tropical instability waves over the recent three decades 

Minyang Wang, Shang-Ping Xie, Hideharu Sasaki, Masami Nonaka, and Yan Du

Tropical instability waves (TIWs), one of the most prominent mesoscale oceanic phenomena in the tropical Pacific, play important roles in climate and ecosystem. Due to limited observations and the difficulty in estimating equatorial current velocity, long-term changes in TIWs remain unknown.

 

Rather than the geostrophic equilibrium (Bonjean and Lagerloef, 2002), the TIW currents exhibit a momentum balance between inertial forces (local accelerations and advections), the Coriolis force and the pressure gradient force. Using a shallow water diagnostic model that retains the inertial forces, we have produced the TIW surface currents since 1993 based on the satellite altimetry sea surface height observations. The results have been well validated with moored observations of ocean velocities in TAO array (Wang et al., 2020, https://doi.org/10.1175/JPO-D-20-0063.1).

 

The satellite altimetry-derived TIW currents (1993-2021) have shown that TIWs have strengthened during this period, with their eddy kinetic energy (EKE) increasing by 12% per decade (~10 J m-3 per decade). The trend has been corroborated by other three independent datasets: satellite-observed sea surface temperature (1982-2021), moored currents from TAO (1980s-2020), and a global eddy-resolving ocean circulation model data (OFES2, 1958-2021). They consistently imply that the intensification is concentrated on the equatorial Yanai-mode TIWs. EKE budget based on OFES2 model data suggests that the increased EKE is attributed to the increased barotropic (primary) and baroclinic (secondary) instabilities. The former is due to the strengthened south equatorial currents (SEC), and the latter is due to the decreased mixed layer stratification and increased equatorial buoyancy fronts. The underlying mechanism is an enhanced cross-equatorial asymmetric warming in the eastern tropical Pacific since the 1990s that forces the changes in the equatorial multiscale ocean dynamics. As a feedback effect on the heat budget of cold tongue SST, the intensified TIWs lead to increased eddy dynamic heating effects of ∼70% since the 1990s near the equator, with implications for predicting and projecting tropical Pacific climate changes. (https://doi.org/10.1038/s41558-023-01915-x)

How to cite: Wang, M., Xie, S.-P., Sasaki, H., Nonaka, M., and Du, Y.: Intensification of Pacific tropical instability waves over the recent three decades, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5858, https://doi.org/10.5194/egusphere-egu25-5858, 2025.

EGU25-6892 | Orals | OS1.9

Mechanical Air-Sea Interactions at submesoscale and Wind Rolls Scales 

Lionel Renault, Enesto Rodriguez, Carlos Conejero, Igor Uchoa, Patrick Marchesiello, Marcela Contreras, and Jacob Wenegrat

In this study, we use in situ observations and high-resolution coupled ocean-atmosphere simulations to investigate the mechanical coupling between the ocean and the atmosphere (referred to as Current Feedback, CFB) at the oceanic submesoscale (O(10 km)) and wind roll scales. First, we show that while the CFB remains active at the submesoscale with a stronger effect on the surface stress during the winter, its effect on submesoscale energetics is weaker than at the mesoscale. This effect is further weakened by energy contributions from thermal feedback and the highly transient nature of submesoscale flow. In addition, using in situ observations from DopplerScat and very high resolution (dx = 80 m) coupled simulations, we show that wind rolls can obscure the imprint of surface currents on surface stress and low-level winds. This interaction induces an energy transfer from the atmosphere to the ocean that overwhelms the energy transfer from submesoscale currents to the atmosphere, and generates currents coherent with the wind rolls down to 20 m depth.

How to cite: Renault, L., Rodriguez, E., Conejero, C., Uchoa, I., Marchesiello, P., Contreras, M., and Wenegrat, J.: Mechanical Air-Sea Interactions at submesoscale and Wind Rolls Scales, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6892, https://doi.org/10.5194/egusphere-egu25-6892, 2025.

EGU25-6934 | ECS | Posters on site | OS1.9

Shallow open-ocean convection in the Weddell Sea: A case study using observations and modelling techniques 

Rowan Brown, Alexander Haumann, Martin Losch, Carsten Rauch, and Markus Janout

Water mass transformations in the Southern Ocean serve as a lynchpin in the global overturning circulation. Among them, the transformation of Circumpolar Deep Water into Antarctic Winter and Surface Water is uniquely critical for the export of Intermediate Waters north of the Polar Front, the exchange of carbon dioxide between the atmosphere and the subsurface ocean, and the upwards flux of oceanic heat, which inhibits sea ice growth. However, our understanding of the processes responsible for the upwelling of Circumpolar Deep Water and its destruction remains incomplete. We hypothesize that shallow open-ocean convective plumes, only extending into or just below the pycnocline, are underrepresented in both the observational record and in global Earth System Models (ESMs), due to their elusive spatial and temporal scales and the hydrostatic approximation made by all ESMs. Therefore, they play a hitherto undervalued role in setting the water mass structure of the Southern Ocean. We present evidence from a unique year-round upper ocean mooring in the Weddell Sea of a shallow open-ocean convective plume extending into the pycnocline during winter 2021. Using the MITgcm ocean model, we simulate an analogous plume in both hydrostatic and non-hydrostatic configurations. Preliminary results suggest that the conditions necessary to form such plumes can be expected with some regularity in the Weddell Sea. We also note differences between the non-hydrostatic and hydrostatic simulations, highlighting the expected biases associated with the hydrostatic approximation in ESMs.

How to cite: Brown, R., Haumann, A., Losch, M., Rauch, C., and Janout, M.: Shallow open-ocean convection in the Weddell Sea: A case study using observations and modelling techniques, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6934, https://doi.org/10.5194/egusphere-egu25-6934, 2025.

Metre-scale boundary layer turbulence and kilometer-scale submesoscale mixed layer eddies play crucial roles in upper ocean stratification. It is well established that the former generates significant vertical fluxes that mix the upper ocean, while the latter acts to restratify it. However, the interaction between these two multi-scale processes is not well understood, particularly when atmospheric forces are non-negligible. MPAS-Ocean was firstly used to investigate the influence of boundary layer turbulence on submesoscale eddy-induced restratification under various initial conditions. Two parametrizations K-Profile Parametrization (KPP) and k-ε were used to represent different forms of turbulence-induced destratification under the same forcing conditions. Comparison analysis was carried out by comparing the resulting submesoscale eddy-induced restratification. Among all cases, KPP exhibited a larger magnitude of vertical buoyancy flux than k-, indicating stronger turbulence-induced destratification. This enhanced destratification can lead to more intense submesoscale eddy-induced restratification, which largely compensates the turbulence-induced destratification. Furthermore, the value of the mixed layer eddy-induced streamfunction strongly depends on the strength of boundary layer turbulence, suggesting that parameterizations of these two processes may need to consider their interactions. To further explore the bidirectional interactions between these two processes, we are currently employing large-eddy simulation to resolve both. A spatial filter is used to separate the flow into submesoscales and small-scale turbulence. Preliminary results of the large eddy simulations, aiming to elucidate the interactions between these two processes, will be discussed.

How to cite: Jiang, X. and Li, Q.: interaction between boundary layer turbulence and submesoscale mixed layer eddies and its influence on upper ocean stratification, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7745, https://doi.org/10.5194/egusphere-egu25-7745, 2025.

EGU25-8009 | ECS | Orals | OS1.9

AMOC sensitivity to air-sea fluxes parametrization 

Clément Dehondt, Pascale Braconnot, Sebastien Fromang, and Olivier Marti
The Atlantic Meridional Overturning Circulation (AMOC) is a large scale circulation of about 18 Sv and 1.2 PW at 26°N characterized by upper waters flowing northward, losing heat and becoming cold deep waters before flowing back southward. The Deep Water Formation (DWF) and the Subpolar gyre circulation are key aspects of AMOC intensity [1] but strongly depend on air-sea fluxes, thus the need to quantify their influence.

To do so, we compare 5 air-sea fluxes parametrizations within the IPSL General Circulation Model (GCM) [2] based on the new DYNAMICO atmospheric dynamical core [3] and the ocean engine NEMO [4]. We show that the spread in AMOC is more than 2 Sv, confirming the high sensitivity to air-sea fluxes. Furthermore, we manage to explain these discrepancies by assessing (i) winter time buoyancy fluxes in DWF area and (ii) subtropical and subpolar gyres intensity which drives the circulation. We also analyse the ocean-atmosphere feedbacks (mainly wind and sea surface temperature) that may be responsible for changes in AMOC, hence paving the way to a better representation in GCMs.
 
 
[1] Buckley, M. W. and J. Marshall (2016), Observations, inferences, and mechanisms of Atlantic Meridional Overturning Circulation variability: A review, Rev. Geophys., 54, 5–63, doi:10.1002/2015RG000493.
 
[2] Boucher O., Servonnat, J., Albright, A. L., Aumont, O., Balkanski, Y., Bastrikov, V., et al. (2020). Presentation and evaluation of the IPSL‐CM6A‐LR climate model. Journal of Advances in Modeling Earth Systems, 12, e2019MS002010. https://doi.org/10.1029/2019MS002010
 
[3] Dubos, T., Dubey, S., Tort, M., Mittal, R., Meurdesoif, Y., and Hourdin, F.: DYNAMICO-1.0, an icosahedral hydrostatic dynamical core designed for consistency and versatility, Geosci. Model Dev., 8, 3131–3150, https://doi.org/10.5194/gmd-8-3131-2015, 2015.
 
[4] “NEMO ocean engine”, Scientific Notes of Climate Modelling Center, 27 — ISSN 1288-1619, Institut PierreSimon Laplace (IPSL), doi:10.5281/zenodo.1464816

How to cite: Dehondt, C., Braconnot, P., Fromang, S., and Marti, O.: AMOC sensitivity to air-sea fluxes parametrization, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8009, https://doi.org/10.5194/egusphere-egu25-8009, 2025.

EGU25-9247 | Orals | OS1.9

Dynamics of sea breezes: Analysis of recent events in Southwest Spain 

Esther Luján-Amoraga, Carlos Román-Cascón, Marina Bolado-Penagos, Pablo Ortiz-Corral, Juan Alberto Jimenez-Rincón, Alfredo Izquierdo, Miguel Bruno, and Carlos Yagüe

Coastal breezes are mesoscale meteorological phenomena primarily driven by the thermal contrast between land and sea surfaces, creating a dynamic system that influences local circulation. These phenomena, common in coastal regions, have a significant impact on various environmental aspects, such as regulating extreme temperatures, transporting atmospheric pollutants, and modifying coastal surface ocean currents. This study aims to characterize the sea breeze system along the southwest coast of Spain, using a combination of observational data to provide a more detailed understanding of these phenomena in the region.

The analysis of sea breeze events focused on the summers of 2023 and 2024, using data obtained from coastal meteorological stations and radiosondes launched specifically in the study area to gather vertical information on the breezes. To detect breeze events, an objective algorithm based on the work of Borne et al. (1988), Arrillaga et al. (2018), and Román-Cascón et al. (2019) was used. This algorithm facilitated the identification of breeze events based on atmospheric conditions, providing a basis for further analysis.

A key contribution of this study is the proposal of a new classification of breeze types, enabling a more accurate characterization of different breeze events, by considering variables such as intensity, duration, and associated synoptic conditions. Furthermore, statistics of the recorded events are presented, offering a deeper insight into the frequency, intensity, and temporal characterization of breezes in the study area. The study also explored the relationship between turbulent variables during breeze events and different tidal moments, which is particularly relevant due to the large intertidal zone affecting one of the stations used. This observational approach enhances the understanding of the coastal breeze system in the study area and contributes to the broader knowledge of these phenomena.

How to cite: Luján-Amoraga, E., Román-Cascón, C., Bolado-Penagos, M., Ortiz-Corral, P., Jimenez-Rincón, J. A., Izquierdo, A., Bruno, M., and Yagüe, C.: Dynamics of sea breezes: Analysis of recent events in Southwest Spain, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9247, https://doi.org/10.5194/egusphere-egu25-9247, 2025.

Interannual variability of surface mixed-layer near-inertial energy (NIE, representing the intensity of near-inertial waves) in the South China Sea and western North Pacific (WNP) is investigated using satellite-tracked surface drifter data set. It is found that NIE in the study region correlates negatively with El Niño-Southern Oscillation (ENSO) with a correlation coefficient of R = −0.44 and a time lag of 5 months, mainly because the variation of local wind stress lags behind El Niño by 4 months. By separating summer and winter seasons, the correlation is significantly improved. The summer NIE correlates positively with El Niño (R = 0.62), since tropical cyclones over the WNP tend to be stronger and longer-lived during the El Niño developing phase. The winter NIE correlates negatively with El Niño (R = −0.65), since the winter monsoon is weakened by the ENSO-related WNP anomalous anticyclone. This is the first time that interannual variability of NIE is studied by direct current velocity observations. 

How to cite: lu, H.: Interannual Variability of Near-Inertial Energy in the SouthChina Sea and Western North Pacific, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10164, https://doi.org/10.5194/egusphere-egu25-10164, 2025.

Near-inertial internal waves (NIWs) are among the primary drivers of turbulence that sustains the ocean stratification. To propagate downward into the ocean interior, NIWs typically need horizontal scales L∼100 km. Therefore, it is commonly held that NIWs generated by basin-scale midlatitude storms depend on refraction by background vorticity gradients to become horizontally compact and then propagate into the thermocline. This contrasts with NIWs generated by tropical cyclones (TCs), which can rapidly propagate downward regardless of background ocean conditions. Here, we study the upper ocean response to midlatitude storms and TCs using a dynamical framework whose equations of motion are written in terms of vorticity and divergence rather than velocity vectors. We show that patterns of wind stress curl and convergence that are inherently linked to atmospheric convection necessarily generate NIWs that are horizontally compact and can induce substantial downward energy fluxes within the first inertial cycle after storm passage. The vorticity-divergence dynamical framework elucidates this because it allows us to account for spatial wind patterns even when solving motion linearly and for a single point in space. With this, we argue that the morphology of mesoscale convective systems allows them to drive downward propagation of NIWs in their wakes, whether ocean storms take the shape of a TC or a midlatitude storm.

How to cite: Brizuela, N. and D'Asaro, E.: Morphology of atmospheric convective systems facilitates rapid transmission of near-inertial energy into the ocean thermocline, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11271, https://doi.org/10.5194/egusphere-egu25-11271, 2025.

EGU25-11742 | Posters on site | OS1.9

Two-particle dispersion in the Gulf of Gabès using a high resolution nested ocean model  

Maher Bouzaiene, Milena Menna, A. Fehmi Dilmahamod, Damiano Delrosso, Simona Simoncelli, and Claudia Fratianni

Measuring relative dispersion in coastal ecosystems is important for both ocean health and society. Submesoscale dynamics interacting with mesoscale eddies influence mixing processes and phytoplankton blooms dispersion. Two-particle dispersion statistics over an initial spatial scale (0.7 - 1 km) are analysed in the Gulf of Gabès (central-southern Mediterranean Sea) using a high-resolution ocean model through a multiple nesting approach. The model is forced by ERA5 atmospheric fields, while the lateral boundary conditions and initial conditions are provided by daily fields from a Mediterranean Sea reanalysis. The analysis focuses on the turbulent fluid aspects of phytoplankton dispersion in coastal areas under bloom and non-bloom conditions. The results are presented in terms of kurtosis (normalized fourth moment of the pair separation distances), relative diffusivity (particles’ spreading velocity) and time scale-dependent pair separation rate (pair velocity scales normalized by separation distance). At the submesoscale (0.7 – 2km), the non-local exponential regime is absent in both bloom and non-bloom conditions, where the dispersion is locally driven by energetic submesoscale structures. For scales ranging 2-15 km, the two-particle statistics follow the theoretical Richardson regime, which is well detected in the case of a bloom. This regime implies the presence of an inverse energy cascade range where energy is transferred from small to large scales. The diffusive regime is absent for all scales and in both bloom and non-bloom conditions.

How to cite: Bouzaiene, M., Menna, M., Dilmahamod, A. F., Delrosso, D., Simoncelli, S., and Fratianni, C.: Two-particle dispersion in the Gulf of Gabès using a high resolution nested ocean model , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11742, https://doi.org/10.5194/egusphere-egu25-11742, 2025.

EGU25-12896 | Posters on site | OS1.9

Near surface bubble, gas and flow measurements during the Bubble Exchange in the Labrador Sea (BELS) cruise – early results 

Helen Czerski, Intesaaf Ashraf, Ian Brooks, and Steve Gunn

The bubbles formed by breaking waves are thought to play an important role in increasing gas transfer across the atmosphere-ocean surface during high wind conditions (>15 m/s).  However, real world data on near-surface bubbles with sufficient resolution in space, time and bubble size to understand exactly how the transfer mechanisms work is rare. In addition, there are almost no data showing the relationship between bubble size distributions and the local flow and gas saturation conditions, although data from the HiWinGS cruise suggests that these structures could be very important for gas transfer. The BELS project data was collected during five weeks in November/December 2023, and includes tracer-based gas flux measurements, physical oceanography, and ocean chemistry.  Hourly averaged wind speeds were 5-30 m/s, with maximum significant wave height of 11 m.  Here, we will present early results from the part of the project monitoring near-surface bubbles and their relationship to flow patterns and dissolved gas concentrations in the top five metres of the ocean. Data will be presented from a free-floating buoy carrying specialised bubble cameras at 1m and 3m, ADCPs and oxygen optodes. We will show measured bubble size distributions, and the spatial relationship of these bubbles to Langmuir circulation patterns and dissolved oxygen concentrations. We will also present an early analysis of the relationships between gas carried by both the water itself and the bubbles, and how this relates to the advection of these two gas reservoirs in the top few metres of the ocean.  

How to cite: Czerski, H., Ashraf, I., Brooks, I., and Gunn, S.: Near surface bubble, gas and flow measurements during the Bubble Exchange in the Labrador Sea (BELS) cruise – early results, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12896, https://doi.org/10.5194/egusphere-egu25-12896, 2025.

EGU25-13975 | Orals | OS1.9

Assessment of satellite-derived sea surface salinity using in-situ measurements in the Southeast Asia 

Kaushik Sasmal, Sumit Dandapat, Xingkun Xu, Pavel Tkalich, Bijoy Thompson, Rajesh Kumar, Kalli Furtado, and Hugh Zhang

Advances in satellite microwave remote sensing have demonstrated an unprecedented capability to observe global ocean sea surface salinity (SSS) from space since 2009. Satellite-based SSS observations provide a unique monitoring capability for the interfacial water exchanges between the atmosphere and the upper ocean, as well as salinity redistribution due to climate and global water cycle variability, and land-ocean interactions.

Satellite measurements of sea surface salinity (SSS) started in November 2009 with the Soil Moisture and Ocean Salinity (SMOS) mission launched by the European Space Agency (ESA). The Aquarius/SAC-D, launched in June 2011 by NASA and the Argentinean Space Agency (CONAE), was the first satellite mission designed to measure SSS. Meanwhile, the Soil Moisture Active and Passive (SMAP) was launched by NASA in January 2015, and it provides SSS as a derived product. SMAP is configured with a larger swath coverage, providing a higher spatial resolution (~40 km) than that (~100 km) in Aquarius.  

Satellite remote sensing of SSS encounters many challenges, such as contamination of microwave signals near coastal areas or dependance of SSS accuracy on the quality of temperature and wind speed measurements. As such, the satellite-derived SSS data needs to be validated against in-situ measurements.

Here we used in-situ measurements of salinity and temperature from ARGO data for three oceanic basins i.e., Bay of Bengal (BOB), South China Sea (SCS), and Western North Pacific Ocean (WNPAC). The ARGO data from Sep 2011 to Dec 2022 were utilized for analysis due to the consistency of the period with the available satellite-derived salinity data. The number of ARGO profiles varies significantly among these three oceanic basins with the largest profiles available in the WNPAC and the least number of profiles in the SCS.

ARGO SSS climatology, although available at a coarser resolution than the satellite-derived SSS, captured the spreading of the low salinity water in the BOB during Oct-Dec. This feature is consistent with the satellite-derived SSS spatial distribution. For the BOB, the agreement between ARGO and satellite SSS data is reasonably good with an RMSE of 0.58 psu. In comparison, the SCS and WNPAC achieve RMSE of 0.22 psu and 0.14 psu, respectively. It should be noted that the number of near-surface ARGO observations is much higher in the WNPAC (37,207) compared to that in the BOB (15,305) and in the SCS (9,722) from Sep 2011 to Dec 2022. The BOB reveals strong seasonality and the largest variation in SSS from ~25-35 psu. Whereas, the SCS and WNPAC recorded variations in the range ~32-35 psu. The SCS and WNPAC exhibit freshening and salinification in specific years. The monthly mean SSS from ARGO and satellite data are highly correlated and show consistent variation in salinity in all three oceanic basins. Therefore, the satellite-derived SSS data could provide great insight for understanding ocean dynamics, circulation, water cycle, and could be useful for validating ocean models.  

How to cite: Sasmal, K., Dandapat, S., Xu, X., Tkalich, P., Thompson, B., Kumar, R., Furtado, K., and Zhang, H.: Assessment of satellite-derived sea surface salinity using in-situ measurements in the Southeast Asia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13975, https://doi.org/10.5194/egusphere-egu25-13975, 2025.

EGU25-14006 | ECS | Posters on site | OS1.9

Relating surface signatures to modeled turbulence dynamics in open channel flow 

Boqi Tian, C. Chris Chickadel, and Ramsey R. Harcourt

In open channel flow (OCF), expressions and patterns at the water surface may represent underwater turbulent phenomena. In this study, we seek to connect the surface signatures with the turbulence beneath it through the prediction of the time and length scales of turbulent structures in second moment closure (SMC) models. In the simplest scenario, the unforced free surface OCF is driven by a uniform horizontal pressure gradient and the only source of turbulence is the bottom shear. Working with Neumann surface boundary conditions for turbulence quantities, the traditional ‘return-to-isotropy’ for turbulent kinetic energy (TKE) components is modified to decay – in the absence of local TKE production – to a specified anisotropy profile as a function of depth below the surface, rather than to isotropy. This gives rise to distinct vertical and horizontal length scales, formed from the TKE components and the turbulence decay timescale. It also results, through changes in the algebraic closure solution, in a modification of vertical diffusivity consistent with more ad-hoc proposals in other studies to address excessive flux predictions using depth-dependent damping functions. An examination of results from these model changes is presented for weak equilibrium k - ε SMC models. The weak equilibrium k - ε SMC model solves for turbulent second moments by combining prognostic equations for TKE (k) and dissipation (ε) with an algebraic model to obtain eddy viscosity and diffusivity. SMC predictions for TKE components, dissipation, and horizontal turbulent length scales at the free surface are compared with observations obtained in a tidally modulated river, as well as with published results from OCF lab experiments and direct numerical simulations.

How to cite: Tian, B., Chickadel, C. C., and Harcourt, R. R.: Relating surface signatures to modeled turbulence dynamics in open channel flow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14006, https://doi.org/10.5194/egusphere-egu25-14006, 2025.

EGU25-14246 | ECS | Orals | OS1.9

Spatial Extent and Variability of Equatorial Deep-Cycle Turbulence in the Pacific Cold Tongue 

Jofia Joseph, Anna-Lena Deppenmeier, Daniel B Whitt, Frank O. Bryan, William S. Kessler, LuAnne Thompson, and Elizabeth Thompson

Deep-cycle turbulence (DCT) is a critical mechanism driving vertical mixing in the equatorial Pacific, playing a pivotal role in modulating heat and nutrient transport within the Pacific Cold Tongue. DCT arises from diurnal variations in stratification and shear, leading to turbulence that extends below the mixed layer. DCT generates significant heat fluxes into the ocean, averaging O(100 W m⁻²) and peaking at ~1000 W m⁻² during nighttime bursts, which contribute to surface cooling and thermocline warming. This process helps maintain cool sea surface temperatures (SSTs) and net heat uptake in the eastern Pacific Cold Tongue, influencing SST dynamics on interannual, seasonal, and subseasonal timescales. These dynamics significantly impact air-sea interactions, as DCT regulates the exchange of heat, momentum, and gases, which play a critical role in shaping tropical weather patterns and global climate variability.

 Despite previous studies elucidating the temporal variability and mechanisms of DCT on the equator, its spatial extent and variability across the equatorial Pacific remain poorly understood due to limited observations.

This study examines the spatial and temporal variability of DCT in the Cold Tongue region using Large Eddy Simulations (LES), which explicitly resolve sub-grid-scale mixing processes. The LES cover a meridional array of seven latitudinal points (1.5°S to 4.5°N) along 140°W and a zonal array spanning the central to eastern Pacific (165°W to 100°W) along the equator during contrasting periods influenced by Tropical Instability Waves (TIWs) and the seasonal cycle. Complementary hourly turbulence outputs from a 20-year MITgcm simulation are utilized to examine parameterized turbulence at these locations, enabling a comparison between sub-grid-resolved turbulence in LES and parameterized turbulence in the MITgcm.

Diurnal composite analyses reveal that parameterized turbulence in the MITgcm overestimates diapycnal heat flux compared to LES-resolved turbulence. The relationship between Richardson number, shear, stratification, and mixing is explored to understand the transition from the marginally stable regime near the equator (0°N, 140°W) to more stable conditions farther from the equator. Preliminary findings illustrate spatial asymmetries in mixing-related variables, with notable differences between the northern and southern hemispheres. These results highlight the need for further exploration of hemispheric asymmetries and their implications for mixing processes.

This study sets the stage for a comprehensive evaluation of mixing representation in the Pacific Cold Tongue region across diurnal to longer timescales, leveraging a hierarchy of model outputs, from LES to regional and global high-resolution simulations.

How to cite: Joseph, J., Deppenmeier, A.-L., B Whitt, D., O. Bryan, F., S. Kessler, W., Thompson, L., and Thompson, E.: Spatial Extent and Variability of Equatorial Deep-Cycle Turbulence in the Pacific Cold Tongue, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14246, https://doi.org/10.5194/egusphere-egu25-14246, 2025.

EGU25-14275 | ECS | Posters on site | OS1.9

Ocean-atmosphere coupling regimes in the tropical area 

Ruyan Chen

Tropical ocean-atmosphere coupling plays a pivotal role in regulating the global climate system. Variability and mechanisms of the coupling exhibit significant regional differences due to variations in the background states and thermodynamic processes across the tropical basins. While previous studies mostly focused on the specific time scales and localized regions, a broader view of the tropical air-sea coupling “picture” remains incomplete. This project first utilizes an energy balance model of the coupled ocean-atmosphere system to diagnose the coupling characteristics for each tropical grid point across timescales through the “heat flux—sea surface temperature” relationship. Subsequently, a clustering algorithm is used to classify spatial differences into distinct coupling regimes. Finally, decomposition of the flux calculation is applied to identify critical variables and processes underlying each regime. This approach progressively reveals the mechanisms behind the regional differences in tropical ocean-atmosphere coupling features. Our findings also highlight that current high-resolution climate models still face challenges in accurately reproducing the coupling characteristics of some regimes, which would further limit the accuracy of climate simulation and prediction.

How to cite: Chen, R.: Ocean-atmosphere coupling regimes in the tropical area, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14275, https://doi.org/10.5194/egusphere-egu25-14275, 2025.

EGU25-14613 | ECS | Orals | OS1.9

Resolving Langmuir Turbulence in a Coupled Wind-Wave System 

Yankun Liu and Qing Li

Langmuir turbulence, arising from the nonlinear interaction between surface gravity waves and wind-driven shear currents, significantly contributes to ocean mixing and the air-sea transfer of mass, momentum, and energy. Previous studies have either prescribed surface wind stress in single-phase flow simulations or left surface waves indeterminate in two-phase flow simulations. To better understand the generation and evolution of Langmuir turbulence, and to quantify the momentum and energy transfer across the air-sea interface, a series of two-phase wave-resolved direct numerical simulations are conducted across various Langmuir numbers. In these simulations, fully developed pressure gradient-driven turbulence on the air side is acted upon prescribed surface gravity waves. The results reveal characteristic structures of Langmuir cells at varying scales, including pairs of counter-rotating vortices and elongated streamwise streaks on the water surface. By decomposing flow velocity into mean current, wave orbital motion, and turbulence fluctuation, the impact of wave-induced phase-dependent strain on underlying turbulence and the enhancement of streamwise vorticity are analyzed in detail. Additionally, the momentum flux across the air-sea interface is calculated and its transfer mechanism is discussed, providing insights for parameterization in climate models.

How to cite: Liu, Y. and Li, Q.: Resolving Langmuir Turbulence in a Coupled Wind-Wave System, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14613, https://doi.org/10.5194/egusphere-egu25-14613, 2025.

EGU25-16290 | ECS | Orals | OS1.9

The role of small-scale ocean mixing processes in regional sea surface temperature 

Audrey Delpech and Anne-Marie Tréguier
The advances of numerical performances over the last decades have opened the way for km-scale climate modelling, which not only improve the representation of the state of the climate globally, but also allows to downscale climate information at a local scale where climate adaptation strategies are decided. In this context, it is interesting to evaluate the performance of such models at a regional scale.
In this study, we evaluate the capabilities of km-scale coupled climate simulations delivered by the EERIE (European Eddy-RIch Earth system models) project on the North Atlantic coastal shelfs in the representation of sea surface temperature and air surface temperature. Our findings suggest that eddy-rich coupled simulations can alleviate some of the large-scale biases found at coarser resolution but at the same time points out towards persistent model biases at local-scale due to unresolved or poorly parameterized mixing processes. We subsequently evaluate the nature and impact of unresolved oceanic mixing processes in climate models on the sea surface temperature mean state, variability and extremes.
 

How to cite: Delpech, A. and Tréguier, A.-M.: The role of small-scale ocean mixing processes in regional sea surface temperature, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16290, https://doi.org/10.5194/egusphere-egu25-16290, 2025.

EGU25-16435 | Posters on site | OS1.9

Three-dimensional Ocean Surface Layer Response to Rain, Wind Bursts and Diurnal Heating 

Lars Umlauf, Mira Schmitt, Knut Klingbeil, and Radomyra Shevchenko

In the tropical ocean, diurnal heating and the formation of atmospheric convection cells associated with local precipitation events, cold pools and wind bursts, have been shown to impact air-sea exchange and the structure of the ocean surface layer. Here, we use a high-resolution regional ocean model, forced by an atmospheric Large Eddy Simulation (LES) that explicitly resolves these processes in a realistic scenario in the tropical north-east Atlantic Ocean, to study their impact on the ocean surface layer and parameterized air-sea fluxes.  We find that in our study area, located in the trade wind zone, the oceanic heat loss is, unexpectedly, reduced in the presence of cold pools by on average 30 W m-2 due to the higher air humidity, weaker mean winds, and increased cloud cover. Our results also show that the total non-solar heat flux is dominated by the diurnal cycle of the trade winds, rather than by diurnal heating. In the ocean surface layer, local wind bursts, rain layers, and cloud shading induce a strong lateral variability of Diurnal Warm Layers (DWLs), questioning the local applicability of available DWL bulk parameterizations. From a series of numerical tracer experiments, we identify a new shear-dispersion mechanism, induced by the diurnal jet, that is reflected in an extreme anisotropy of horizontal dispersion with diffusivities of order 10-100 m2 s-1. These findings are likely relevant also in other regions in the trade wind zone.

How to cite: Umlauf, L., Schmitt, M., Klingbeil, K., and Shevchenko, R.: Three-dimensional Ocean Surface Layer Response to Rain, Wind Bursts and Diurnal Heating, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16435, https://doi.org/10.5194/egusphere-egu25-16435, 2025.

EGU25-17338 | ECS | Posters on site | OS1.9

Leveraging automatic differentiation for calibrating vertical mixing parameterizations  

Gabriel Mouttapa, Julien Le Sommer, Emmanuel Cosme, Anne Durif, Bruno Deremble, Alexandre Legay, and Gregory LeClaire Wagner

Fine-scale turbulence in the upper ocean boundary layer (OSBL) governs ocean surface stratification, and vertical exchanges of heat, momentum and matter in the ocean, which are key in the response of the oceans to changing environmental conditions. However, these turbulent processes are not explicitly represented in ocean models and their parameterization remains a significant source of uncertainty in climate models and operational prediction systems. Increasingly, systematically leveraging diverse data sources is becoming standard practice for developing and assessing OSBL parameterizations. Over the past years, data-driven automated procedures have for instance been used for calibrating the parameters of physics-based models, for developing parameterizations embedding ML components, and for proposing pure ML-based parameterizations of OSBL processes. 

This study explores the advantages of the emerging paradigm of differentiable programming for the calibration of OSBL parameterizations . We developed a benchmark tool, Tunax, implemented in JAX, a differentiable framework for Python. This benchmark includes a fully differentiable single-column model with various possible OSBL parameterizations, alongside a calibration module which tunes the coefficients of these parameterizations against a reference database. The differentiability of the model enables the application of variational techniques for parameter calibration. The reference database is a collection of  Large Eddy Simulations (LES) covering a range of typical physical conditions.

Here, we focus on the k-ε closure (Umlauf and Burchard, 2005), widely used in global ocean circulation models, and calibrate its parameters using a dataset of LES. These simulations have been designed to model the evolution of the oceanic mixed layer under various surface conditions (wind, heat fluxes and rotation). This work highlights the potential of differentiable calibration techniques to address uncertainties inherent to turbulence closures by enabling more flexible and data-informed parameterizations. Although this approach does not yet consistently outperform traditional calibration methods, it provides a promising avenue for reducing model biases associated with sub-grid scale parameterizations.

 

How to cite: Mouttapa, G., Le Sommer, J., Cosme, E., Durif, A., Deremble, B., Legay, A., and LeClaire Wagner, G.: Leveraging automatic differentiation for calibrating vertical mixing parameterizations , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17338, https://doi.org/10.5194/egusphere-egu25-17338, 2025.

There is a large number of mesoscale eddies in the ocean, which play a significant role in ocean circulation and climate change. Recent studies have indicated that mesoscale eddy activity in most regions will become more active under the influence of global warming, but changes in the characteristics of these eddies remain unclear. This study utilizes satellite observational data and reanalysis datasets, focusing on the Agulhas Leakage region, which is rich in mesoscale eddies and has become a research hotspot due to its unique geographical position. The study finds that the changes in the characteristics of anticyclonic eddies in this region are related to variations in the Atlantic Meridional Overturning Circulation (AMOC). Some of the eddy characteristics exhibit dynamic adjustments, with a turning point around 2005, which may be associated with sea temperature differences between the South Indian Ocean and the South Atlantic, as well as changes in the local wind field. The findings of this study will provide insights for future predictions of AMOC variability.

How to cite: Wei, L. and Wang, C.: Why do warm anticyclonic eddies in the Agulhas Leakage undergo dynamic adjustments?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17915, https://doi.org/10.5194/egusphere-egu25-17915, 2025.

EGU25-17994 | Posters on site | OS1.9

On the way towards understanding the effect of sea-water surfactants on gas transfer velocity  

Jacek Piskozub, Violetta Drozdowska, Iwona Wróbel-Niedźwiecka, Karol Kuliński, Przemysław Makuch, Fernando Aguado Gonzalo, Piotr Markuszewski, and Małgorzata Kitowska

Gas flux across the sea surface is proportional to the difference of partial pressure between the sea-water and the overlying atmosphere and also to a parameter called gas transfer velocity k, a measure of the, the measure of efficiency of the gas exchange. Although it depends mostly in in-water and atmospheric turbulence, the usual way to parametrize it is by the wind speed, the source of the turbulence which has the advantage of being easily available from ship base measurements and reanalyses. Unfortunately, measured values of gas transfer velocity at a given wind speed have a large spread in values. It has been long suspected that the coverage of the sea surface with variable amounts of surface-active substances (or surfactants). It has been shown that surfactants may decrease the CO2 air-sea exchange by up to 50%. However the labour intensive methods used for surfactant study make it impossible to collect enough data to map the surfactant coverage or even create a gas transfer velocity parametrization involving a measure of surfactant activity. This is why we decided check the possibility of using optical fluorescence as a proxy of surfactant activity.

 

We are in the third year of a 4-year research grant funded by the Polish National Science Centre, NCN (grant number 2021/41/B/ST10/00946). Our group has previously showed that fluorescence parameters allow estimation the surfactant enrichment of the surface microlayer, as well as types and origin of fluorescent organic matter involved. In order to study their possible usefulness in improving the parametrization of the gas transfer velocity k, we measure from the research ship of the Institute, R/V Oceania, all the variables needed for its calculation, namely CO2 partial pressure both in water (PiCCARO G2101-i) and in air (Licor 7200, semiclose path with heated tube and Licor 7500, open path) as well as vertical flux of this trace gas (with the GiLL WindMaster and WindMaster Pro for 3D air movement needed for eddy correlation) as well as meteorological conditions. The data are used to calculate gas transfer velocity values which are compared to ones calculated literature from parametrization functions. The differences between the two, together with the surfactant fluorescence parameters are be used to test the hypothesis that surfactants are main reason for the “noisiness” of k measurement results and hopefully to improve the k parametrization by adding a surfactant related variable to the wind speed which at present is the sole independent variable of most parametrizations.

 

After 3 years of the project we have data from six Baltic cruises and to three Atlantic ones, of which 2/3 have been already analysed. The poster will present the early results of the project and show progress towards the main goal of the research: finding a reliable optical proxy for surfactant to be used in gas transfer velocity parametrization.

 

How to cite: Piskozub, J., Drozdowska, V., Wróbel-Niedźwiecka, I., Kuliński, K., Makuch, P., Aguado Gonzalo, F., Markuszewski, P., and Kitowska, M.: On the way towards understanding the effect of sea-water surfactants on gas transfer velocity , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17994, https://doi.org/10.5194/egusphere-egu25-17994, 2025.

EGU25-18385 | Posters on site | OS1.9

Characterizing Wind-Generated Waves Using a Color Imaging Slope Gauge (CISG) 

Julián Marcelo Morales Meabe and Martin Gade

Wind-driven waves play a pivotal role in air-sea interactions, influencing processes such as energy dissipation and turbulent mixing. In this study, we employ a Color Imaging Slope Gauge (CISG) to measure surface wave slopes with high spatiotemporal resolution in the linear wind-wave tank at the University of Hamburg. Complementary techniques include a Laser Doppler Velocimetry (LDV) system for point-wise, two-dimensional velocity measurements; a wire gauge and a laser slope gauge for point measurements of wave height and slope, respectively; and an infrared radiometer capable of capturing surface temperature variations. These tools enable the investigation of thermal gradients and their correlation with wave dynamics. 

This research aims to examine the statistical properties of wind-generated waves and reconstruct their three-dimensional profiles to better understand their physical and kinematic behavior. A particular focus is placed on the mechanisms of microbreaking, which contribute to energy dissipation and capillary wave generation. To explore surface tension effects, surfactants are introduced to dampen gravity-capillary waves, allowing for detailed investigations of energy fluxes between wave regimes and the suppression of high-frequency wave components. 

The combined use of slope imaging, velocity measurements, and thermal detection enhances our ability to study the interplay of different physical processes at the air-sea interface. This work lays the groundwork for further investigations of wave behavior under varying environmental conditions. In particular, the findings of this study will provide critical insights into the small-scale processes driving wave dynamics and contribute to improved parameterizations for wave and climate models. 

 

How to cite: Morales Meabe, J. M. and Gade, M.: Characterizing Wind-Generated Waves Using a Color Imaging Slope Gauge (CISG), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18385, https://doi.org/10.5194/egusphere-egu25-18385, 2025.

EGU25-18410 | ECS | Posters on site | OS1.9

Impact of Submesoscale Dynamics and Turbulent Mixing on the Senegalo-Mauritanian Upwelling System 

Marco Schulz, Florian Schütte, Marcus Dengler, and Peter Brandt

Based on a combination of over 20 years of satellite data with extensive in situ measurements from previous research expeditions, an initial step is taken to differentiate the impact of submesoscale processes and turbulent mixing on the Eastern Boundary Upwelling System (EBUS) off Senegal and Mauritania. EBUS are an essential part of the global carbon cycle and are of central importance for the sustainability of economic and food resources. In the tropical Senegalo-Mauritanian EBUS, sea surface temperatures and net primary production exhibits a pronounced seasonal cycle. It is characterized by coastal upwelling in late boreal winter and an abrupt end in late boreal spring with the onset and strengthening of the poleward Mauritania Current. At first glance, the temporal and spatial development follows the annual cycle of the wind stress curl. However, a closer look reveals a more complex picture with a pronounced spatiotemporal heterogeneity, characterized by the influence of (sub)mesoscale eddies and (non-linear) internal tides.

Integrated cross-shelf tidal energy fluxes towards the coast are locally estimated from observations of multiple short-term moorings. Such fluxes should result in increased mixing near the coast, which is in fact supported by assessment of over 800 microstructure turbulence observations. (Internal) tides are known to drive much of the mixing and vertical exchange on a rather narrow coastal strip. Besides, lateral density gradients which were induced by upwelling are regularly subject to conditions favorable for frontogenesis. The associated secondary circulations can induce strong vertical motions and instabilities and export chlorophyll offshore through frontal jets. A snapshot of ship-based measurements of turbulent kinetic energy dissipation rates indicates an order of magnitude larger dissipation on the cold, dense side of the front, whereby surface heat flux is known to play a crucial role. Spatially high-resolution measurements of sea level deflections from the SWOT satellite show considerable variability on scales smaller than 20 km, but the applicability for balanced motions is hampered by the regular occurrence of solitary waves and topographic effects. Given the significance of these observed small-scale processes for the redistribution and alteration in net primary production and expected general changes of submesoscale processes (e.g. due to changing mixed layer depths in the context of global warming), a more precise quantification of their net impact is essential.

Outlook: An interdisciplinary expedition in spring 2025 will supplement the existing data and will use an adaptive sampling strategy, e.g. to tackle the mutual interaction of tides and internal waves with density fronts. Observed tidal fluxes will be interpreted in the context of a high-resolution 3D baroclinic tidal model. These, as well as the work presented, serve as preparatory work for the unprecedented year-round “FUTURO” campaign, which aims to provide a detailed picture of the annual cycle for this important EBUS.

How to cite: Schulz, M., Schütte, F., Dengler, M., and Brandt, P.: Impact of Submesoscale Dynamics and Turbulent Mixing on the Senegalo-Mauritanian Upwelling System, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18410, https://doi.org/10.5194/egusphere-egu25-18410, 2025.

EGU25-18874 | ECS | Orals | OS1.9

Parameterizing Entrainment Induced by Submesoscale Eddies 

Anna Lo Piccolo, Baylor Fox-Kemper, Genevieve Jay Brett, Tomás L. Chor, Jacob O. Wenegrat, and Zhihua Zheng

Submesoscale eddies in the ocean surface layer are known to cause the restratification of the mixed-layer by converting the potential energy stored in the outcropping isopycnals into kinetic energy. Evidence of entrainment and subduction is found associated to submesoscale eddies, suggesting their importance for the biogeochemistry of the global ocean. Submesoscale eddies cannot be resolved in today’s global ocean models and existing parameterizations for baroclinic mixed-layer instabilities (MLIs), which are proven to reproduce the restratification quite well, are not capable to fully capture the vertical exchange of passive tracers across the mixed-layer. In this study, high resolution numerical simulations show the inadequacy of the MLI parameterization of Fox-Kemper, Ferrari, and Hallberg (2008, ‘FFH’) for the entrainment problem. A method for tracer inversion is then used to gain insights on the tracer transport in order to inform the parameterization. Parameter dependence is explored by considering different ocean initial conditions. Finally, the results show that a diffusive (symmetric) component needs to be included to the streamfunction (anti-symmetric) to entirely represent the transport induced by MLIs: the parameterization for entrainment is an update to the FFH parameterization.

How to cite: Lo Piccolo, A., Fox-Kemper, B., Brett, G. J., Chor, T. L., Wenegrat, J. O., and Zheng, Z.: Parameterizing Entrainment Induced by Submesoscale Eddies, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18874, https://doi.org/10.5194/egusphere-egu25-18874, 2025.

In this study, we identify regions across the Mexican Pacific waters where the high-frequency variability of daily sea surface temperature (SST) is diminishing and those in which the warm upper-layer thickness increases, analyzing changes in the upper layers' thermal structure along the tropical Pacific Ocean and their relationship with the variability of the upper-layer thickness in the so-called Warm Pool of the Mexican Pacific. Our results reveal a clear, direct relationship between the thickness increase of the warm, upper-ocean layer and the reduction of the high-frequency SST variability, which are related to the long-term trend of SST and ENSO variability. The implications are enormous since extreme positive SST anomalies and increasing warm, upper-layer thickness are optimal oceanic conditions for forthcoming hurricane development and intensification.

How to cite: Martinez-Lopez, B.: Otis intensification and its relationship to El Niño and Climate Change in the eastern Pacific Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20498, https://doi.org/10.5194/egusphere-egu25-20498, 2025.

Sea spray-mediated heat flux plays an important role in air-sea heat transfer. Heat flux integrated over droplet size spectrum can well simulate total heat flux induced by sea spray droplets. Previously, a fast algorithm of spray-flux assuming single-radius droplets (A15) was widely used since the full-size spectrum integral is computationally expensive. Based on the Gaussian Quadrature (GQ) method, a new fast algorithm (SPRAY-GQ) of sea spray-mediated heat flux is derived. The performance of SPRAY-GQ is evaluated by comparing heat fluxes with those estimated from the widely-used A15. The new algorithm shows a better agreement with the original spectrum integral. To further evaluate the numerical errors of A15 and SPRAY-GQ, the two algorithms are implemented into a coupled CFSv2.0-WW3 system, and a series of 56-day simulations in summer and winter are conducted and compared. The comparisons with satellite measurements and reanalysis data show that the SPRAY-GQ algorithm could lead to more reasonable simulation than the A15 algorithm by modifying air-sea heat flux. For experiments based on SPRAY-GQ, the sea surface temperature at mid-high latitudes of both hemispheres, particularly in summer, is significantly improved compared with the experiments based on A15. The simulation of 10-m wind speed and significant wave height at mid-low latitudes of the Northern Hemisphere after the first two weeks is improved as well. These improvements are due to the reduced numerical errors. The computational time of SPRAY-GQ is about the same as that of A15. Therefore, the newly-developed SPRAY-GQ algorithm has a potential to be used for calculation of spray-mediated heat flux in coupled models.

How to cite: Shi, R. and Xu, F.: Accelerated Estimation of Sea Spray-Mediated Heat Flux Using Gaussian Quadrature, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21343, https://doi.org/10.5194/egusphere-egu25-21343, 2025.

Subduction in the Northwestern Pacific produces North Pacific Subtropical Mode Water (NPSTMW) and constitutes an important branch of the Subtropical Cell. Subduction in the Northwestern Pacific occurs typically during March and April. Based on ocean and atmosphere reanalysis products, the subduction of the NPSTMW is calculated using an Eulerian method. It is found that the averaged subduction time of NPSTMW, weighted by the daily detrainment rate, can vary more than two weeks every year. A composite analysis of the early and the late subduction shows that the subduction time is mostly affected by the strength of the surface zonal wind in the subduction region, which is found to be closely related to the strength and meridional shift of the Aleutian Low in March and April. When the Aleutian Low is stronger (weaker) or shifts southward (northward) in March and April, the surface westerly wind in the subduction region is stronger (weaker), which delays (expedites) the shoaling of the mixed layer and leads to a later (earlier) subduction of the NPSTMW. 

How to cite: Zhang, X. and Xu, F.: The Interannual Variability of North Pacific Subtropical Mode Water Subduction Time Modulated by Aleutian Low, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21345, https://doi.org/10.5194/egusphere-egu25-21345, 2025.

 Accurate precipitation estimation is crucial for hydrological modeling and flood forecasting in the Yangtze River Basin (YRB), China. This study explores the use of machine learning (ML) and deep learning (DL) methods to fuse multi-source precipitation data, including satellite, radar, and ground-based observations. We apply models such as Random Forest (RF), Support Vector Machines (SVM), Convolutional Neural Networks (CNN), and Long Short-Term Memory (LSTM) networks to improve precipitation estimation accuracy. Performance is evaluated using metrics like Mean Absolute Error (MAE) and Root Mean Square Error (RMSE). Our results demonstrate that deep learning models, particularly CNNs and LSTMs, outperform traditional ML methods in terms of accuracy and spatial consistency. This work provides a robust approach to multi-source data fusion, enhancing precipitation monitoring and hydrological applications in the YRB.

How to cite: Chen, T.: Machine Learning and Deep Learning for Multi-Source Precipitation Integration in the Yangtze River Basin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1507, https://doi.org/10.5194/egusphere-egu25-1507, 2025.

EGU25-3311 | PICO | HS7.1

A novel algorithm for remote sensing rainfall retrieval 

Massimiliano Ignaccolo and Carlo De Michele

Dual-polarization radar rainfall rate estimates are based on scaling laws involving the horizontal reflectivity Zh and the ratio between horizontal and vertical reflectivity ZDR. Scaling law parameters obtained from disdrometric observations are highly dependent on the data set used. As a consequence ZR scaling laws do not generalize well. Using the jargon of data science, a ZR scaling law has an accpetable training accuracy and a poor validation accuracy. 

To overcome this limitation, we propose the Formula-R algorithm based on the adoption of the data science parametrization of drop size distributions and its universal shape factors [https://doi.org/10.1175/JHM-D-21-0211.1]. We show, using a worldwide catalog of disdrometric observations, how the Formula-R outperforms the ZR scaling law both in training and validation accuracy. 

The Formula-R algorithm could be used as the foundation of a universal remote sensing retrieval algorithm making the question "which ZR-relationship should we use?" a question of the past.

 

How to cite: Ignaccolo, M. and De Michele, C.: A novel algorithm for remote sensing rainfall retrieval, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3311, https://doi.org/10.5194/egusphere-egu25-3311, 2025.

High resolution rainfall data are essential to quantify small scale and fast hydrological processes. The objective of the paper is to determine temporal variability and spatial patterns of precipitation statistic of one-minute resolution rainfall across Germany. The German Weather Service (DWD) started in 1993 to deploy rain gauges that achieve 1 minute temporal and 0.01 mm volumetric resolution by combining tipping buckets with weigthing (rain[e]H3 by LAMBRECHT meteo GmbH and OTT Pluvio by OTT Hydromet). 345 of those stations all over Germany have data with more than 10 years. For each station empirical cumulative distribution functions (eCDF) of precipitation intensity and dry periods were derived. Data were then aggregated to lower resolutions ranging from 2 min to 4 months. For all aggregation levels we fitted power law, log-normal and Weibull distribution functions and compared the goodness of fit. To determine spatial correlations between stations we extracted intensity and dry period duration at a given frequency from the empirical distribution function and applied a correlation analysis with station longitude, latitude, elevation and total rainfall. Annual and diurnal variations were analysed by fitting a power law to a moving window of data. A 60d segment of the yearly cycle (combining data of all years) and a 4h segment of the daily cycle (combining data of all days) were used. Similar the dependence of the power-law coefficient on temperature was analysed with a moving window of 2.5K width, shifted between -10 to 30°C.

We show that rainfall intensity measured at 1 minute resolution shows a distinct power-law distribution for all stations. The dry period durations instead are not purely power-law distributed. When aggregated, the distribution of the data transitions to lognormal distribution at 15 min aggregation level and to a Weibull distribution from 6 hours onwards. This has significant implication for estimating flood risk and deriving design storm properties as each temporal resolution requires a different statistical distribution to be fitted. We conclude that the mixing of the intensity and dry-period statistic creates this effect. While total rainfall in Germany clearly varies, with high totals in the north-west and lower values in the east, the intensity distribution does not reflect that. We find no significant correlation with longitude, latitude, elevation nor total station rainfall. But the dry-period statistic correlates well. This leads to the conclusion that rainfall intensity statistic is very similar in all of Germany and the difference in recurrence intervals and total rainfall is mostly defined by the dry periods between rain events. The power-law exponent varies annually with a sine curve from -1 to -2 in phase with the annual temperature cycle. It also shows a clear diurnal cycle. It can be expected that those cycles are driven by a strong dependence on temperature. The power-law exponent is close to -3 at 0°C and -1 at 25°C, creating higher intensities at higher temperatures.

How to cite: Frechen, N. and Hinz, C.: One-minute rainfall data reveal temperature dependend seasonal and diurnal variability of the power-law distribution for Germany, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6463, https://doi.org/10.5194/egusphere-egu25-6463, 2025.

EGU25-6983 | ECS | PICO | HS7.1

Multifractal analysis of Liquid Water Content vertical and temporal variability 

Emna Chikhaoui and Auguste Gires

Driven by complex mechanisms, precipitation exhibits extreme variability across scales both in space and time. A clearer insight into this variability can be obtained by exploring multiple parameters, such as the Liquid Water Content (LWC). It is a measurement that quantifies the amount of liquid water available in the atmosphere and as such it provides valuable information about precipitation variability across space and time. While extensive research has focused on analyzing LWC variability at the surface level, studies addressing the vertical variability remain relatively limited. However, it contributes to better understanding of rainfall dynamics, and notably the variability occurring at scales smaller than radar gate.

Within this scope, six months of a Micro Rain Radar PRO (MRR-PRO) observations were gathered in Ecole nationale des ponts et chaussées, Institut Polytechnique de Paris, which is located next to Paris, France. The MRR-PRO is a K-band weather radar that measures hydrometeors fall velocity up to more than 4 kilometers of altitude above its position with a 35 meters spatial resolution and a 10 seconds time step. From collected data and simple assumptions, various quantities related to rainfall drop size distribution including LWC can be derived. The generated data were analyzed to study the spatial and temporal variations of LWC using Universal Multifractals (UM); which is a physically based framework that assesses the variability of geophysical fields across wide ranges of scales with the help of only three parameters with physical interpretation.

In this study, two types of UM analysis are implemented. As a first step, the time series of  LWC at  each altitude is studied. As a second step, vertical profiles of LWC are analyzed and UM parameters characterizing vertical variability are derived. Obtained results and their interpretation in a space-time framework will be presented and discussed.

Authors acknowledge the France-Taiwan Ra2DW project for financial support (grant number by the French National Research Agency – ANR-23-CE01-0019-01).

How to cite: Chikhaoui, E. and Gires, A.: Multifractal analysis of Liquid Water Content vertical and temporal variability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6983, https://doi.org/10.5194/egusphere-egu25-6983, 2025.

The abstraction of precipitation can be defined as the difference between precipitation and runoff. Understanding the dynamics behind water abstraction could provide new insights into hydrological processes and contributes to improved water resource management strategies. This research aims to investigate the phenomenon of water abstraction and critically examine the widely acknowledged assumption that near-surface air temperature is the primary factor influencing the magnitude of water abstraction. The study employs a simplified water balance equation to quantify water abstraction, using observed data from dam catchments in Taiwan, Japan, and South Korea, which span a range of climate types. Data mining techniques, including linear regression and related statistical analyses, are applied to explore the relationship between precipitation and water abstraction across various timescales. Preliminary results indicate that, on a monthly timescale, there is generally a positive correlation between precipitation and water abstraction during the flood season (January–May and November–December) across all catchments. However, the relationship during the dry season (June–October) remains ambiguous. Among the three regions, Japan experiences the highest water abstraction during all seasons, whereas the lowest water abstraction is observed in South Korea during the dry season and in Taiwan during the flood season. On an annual timescale, Japan shows the relative highest water abstraction, while South Korea records the lowest. Notably, our findings diverge from previous research. In Taiwan, particularly during the flood season, an increased incidence of negative water abstraction has been observed. This phenomenon suggests that runoff processes in Taiwan are more influenced by groundwater dynamics than by precipitation.

How to cite: Lu, C. and You, J.-Y.: Observation and Comparison of Precipitation and Water Abstraction Data in Taiwan, Japan, and South Korea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7906, https://doi.org/10.5194/egusphere-egu25-7906, 2025.

EGU25-11476 | ECS | PICO | HS7.1

Retrieval of the hail size number distribution from polarimetric C-band weather radar using double-moment normalization 

Matteo Guidicelli, Alfonso Ferrone, Gionata Ghiggi, Marco Gabella, Urs Germann, and Alexis Berne

Estimating the distribution of hail sizes is crucial for assessing related weather hazards and potential damage to buildings, vehicles and agriculture. In this study, we present a novel technique for estimating the hail size number distribution (HSND) using polarimetric C-band radar data. A generalized additive model (GAM) is employed to estimate two empirical moments of the HSND, which is then reconstructed using double-moment normalization. This approach capitalizes on the relative invariance of the double-moment normalized HSND. The model is trained on data from the Swiss network of automatic hail sensors, spanning from September 2018 to August 2024 and covering three regions of Switzerland particularly prone to hail. Several polarimetric features are extracted from a 3D radar composite that combines observations from all operational Swiss radars. Among the various extracted features, the model selects the echo-top height of 50 dBZ reflectivity value at vertical polarization and the volume of the region with a cross-correlation coefficient rhoHV below 0.97, as these provided the best predictive performance. Radar-derived HSND estimates show good agreement with independent hail sensor observations. Additionally, the model is evaluated through comparisons with photogrammetric drone surveys and crowd-sourced reports of hail. This technique enables high spatio-temporal resolution (1 km and 5 minutes) retrievals of HSND and related metrics, such as kinetic energy. Further ground observations, particularly drone-based, are essential for more comprehensive evaluation of the retrieved HSND.

How to cite: Guidicelli, M., Ferrone, A., Ghiggi, G., Gabella, M., Germann, U., and Berne, A.: Retrieval of the hail size number distribution from polarimetric C-band weather radar using double-moment normalization, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11476, https://doi.org/10.5194/egusphere-egu25-11476, 2025.

Spatial and temporal interpolation methods are generally used for estimation of missing data. Objective selection of control points (sites) with available data in a region for use in spatial interpolation to estimate missing data in space and time is always a challenge. The numerical weights derived through spatial and temporal interpolation approaches attached to data available at different sites have an impact of the estimation of missing data. Parsimonious and robust interpolation models can be developed using schemes that objectively select optimal number of sites and methodologies that eliminate redundant sites and regulate the weights. In this study regularization schemes, mathematical programming model formulations and different feature selection methods used in machine learning field are developed and evaluated for optimal and objective selection of sites for estimation of missing precipitation records. Variants of regularization schemes such as ridge regression, lease absolute shrinkage selection operator (LASSO) and elastic net are experimented. Mixed integer nonlinear optimization programming (MINLP) models with binary variables and multiple feature selection methods are adopted in this work. A case study using precipitation data at several rain gauges in a temperate climatic region of Kentucky, USA is used to demonstrate the benefits of using regularization schemes and optimization with binary variables to select an optimal subset of control points. Results point to improved estimations when these approaches are used for estimation of missing precipitation data.

How to cite: Teegavarapu, R.: Objective and Optimal Spatial Interpolation Approaches for Imputing Missing Precipitation Records, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13245, https://doi.org/10.5194/egusphere-egu25-13245, 2025.

EGU25-13674 | ECS | PICO | HS7.1

 A decade-long analysis of rainfall in Rome based on disdrometer: Rain patterns and Intermittency  

Ravi Shankar Pandey, Natale Alberto Carrassi, Federico Porcù, and Elisa Adirosi

The study presents the first analysis of the rain structure based on 11 years (2013-2023) of continuous 1-min disdrometer data collected by the TC-Clima disdrometer located nearby Rome (Italy). The investigation employs various techniques, including delineating rainfall events based on different minimum inter-event times (MITs), calculating rain rate, mass-weighted mean diameter (Dm), as well as stratiform and convective precipitation classification. The dataset has been pre-processed to filter/remove missing/erroneous information and to ensure unbiased measurements. Seasonal variations showed that autumn had the highest rainfall accumulation (38.8%, 3126.8 mm), despite shorter rain durations (1116.5 hours) compared to winter (1446.5 hours). Winter contributed 28.2% (1986.65 mm) with prolonged rain events of smaller droplets (Dm = 0.98), while summer had the lowest total rainfall (10%, 1329.6 mm) but the highest average rain rate (3.4 mm/h) and largest drops (Dm = 1.39). The difference in drop sizes and rain types across seasons is important, as stratiform clouds, linked to steady rain, were more common in autumn and winter, while convective clouds, associated with intense, short-duration rain, dominated summer. We then focus on rainfall intermittency: the abrupt onset or interruptions of rainfall events. We quantify intermittency by using the intermittency fraction (IFr), i.e., the proportion of time with no rain during an event. Diurnal analysis of IFr revealed significant seasonal differences. Intermittency Fraction peaked between 9am and 2pm, with summer seeing sharp peaks before noon, followed by a rapid decrease in the afternoon. Winter maintained more consistent IFr throughout the day. Rain interruptions have been more frequent in winter, but these breaks were generally short, indicating long-duration, low-intensity rainfall. In contrast, summer had fewer interruptions, but they lasted longer due to intense, short-lived rain. These seasonal differences are robust and appear also by varying the fixed-time averages of the rainfall intermittency. Overall, the longest continuous rain event lasted 19.4hrs, while the longest dry spell was 534.4hrs. The rainfall is an intermittent natural phenomenon whose start and end are defined by rainless intervals referred to as minimum inter-event time, MIT. Intra event rainfall intermittency across various MITs shows higher IFrs at shorter MITs, particularly during summer. Our research also shows that disdrometer measures higher rain amount than conventional rain gauge with highest contrast in summer season. This further underscores the importance of high-resolution rainfall data for accurate predictions. Disdrometers confirmed to be a unique source of reliable and detailed rainfall measurements, which are essential for enhancing resilience against hydro-meteorological challenges such as flooding.

How to cite: Pandey, R. S., Carrassi, N. A., Porcù, F., and Adirosi, E.:  A decade-long analysis of rainfall in Rome based on disdrometer: Rain patterns and Intermittency , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13674, https://doi.org/10.5194/egusphere-egu25-13674, 2025.

Rainfall is known to exhibit extreme variability over wide range of space and time scale, which makes it challenging to characterize, model and even measure. Rainfall measurement devices have observation scales very different from one another ranging from roughly 20 cm in space and few tens seconds (or few minutes) in time for punctual measurement such as disdrometers (or rain gauge), to few hundreds meters in space and few minutes in time for operational weather radars, and up to few kilometres in space and few tens of minutes for satellite data. This very significant observation scale gap between these devices creates a challenge in the comparion simply because of the intrinsic variability of rainfall, even without considering instrumental biases associated to each device.

This work focuses on the impact of the intrinsic rainfall variability on the comparison between punctual (disdrometer or rain gauge) and weather radar rainfall measurement. In order to achieve this, the physically based and mathematically robust framework of Universal Multifractals will be used. It relies on the assumption that rainfall is generated through an underlying multiplicative process. In such framework, the rain rate field can be written as the resolution (defined as the ratio between the outer scale of the phenomenon and the observation scale) to the power of a singularity. This singularity is preserved through scales.

Rainfall data collected in UK and Taiwan are used. These include high-resolution radar composite products and ground gauge records. In the UK, C-band radar composite, Nimrod, at 5-min and 1-km resolutions is used to compare with 1-min rainfall records derived from tipping bucket gauge records, while, in Taiwan, S-band radar composite, QPESUM, at 10-min and 1-km resolutions is used to compare with 10-second disdrometer rainfall records.

The concept of singularity is used to suggest an innovative comparison approach between rainfall measurement devices. More precisely, the local singularity along with the associated uncertainty is assessed using radar data on the range of available space time scales and then compared with the one of disdrometer or rain gauge accounting for the ratio between the observation scales. Results and interpretation of this novel comparison method on the available data will be discussed.

Authors acknowledge the France-Taiwan Ra2DW project (supported by the French National Research Agency – ANR-23-CE01-0019-01 and Taiwan’s National Science and Technology Council – 113-2923-M-002-001-MY4) for partial financial support.

How to cite: Gires, A. and Wang, L.-P.: Multifractal singularity to bridge the scale gap between various rainfall measurement devices, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13715, https://doi.org/10.5194/egusphere-egu25-13715, 2025.

EGU25-15409 | PICO | HS7.1

The wind effects on disdrometer and rain gauges measurements: results from a 4-year long rain series data-set in Pescara and a 10-year long rain series data-set in Calabria (Italy) 

Elisa Adirosi, Leone Parasporo, Luca Baldini, Arianna Cauretuccio, Enrico Chinchella, Tommaso Caloiero, and Luca Lanza

Disdrometers are in-situ, non-catching devices capable of measuring the size and fall velocity (for most models) of each individual hydrometeor (solid or liquid) that enters their measurement volume. These devices are primarily used for research purposes, and their data have applications in fields such as meteorology, climatology, and hydrology. However, their measurements can be influenced by the presence of wind. In this context, one of the objectives of the PRIN project titled “Fostering innovation in precipitation measurements: from drop size to hydrological and climatic scales” is to quantify the accuracy of disdrometers. In this regard, data collected from a Thies Clima disdrometer and wind sensors installed in the city of Pescara serve as a valuable resource for: i) characterizing precipitation, ii) conducting a joint analysis of atmospheric conditions, including wind directionand speed, and iii) evaluating the effect of wind on disdrometer measurements. The dataset covers the period from July 2021 to August 2024, although it includes significant interruptions. This study presents the main characteristics of the site in terms of wind and rain distributions, as well as their joint distributions. Additionally, the effects of wind on disdrometer measurements are quantified in terms of the associated bias on on DSD (Drop Size Distribution) estimation. Results indicate that wind-corrected DSDs differ, on average, by 136.41m−3 ·mm−1 in terms of root mean square error compared to uncorrected DSDs. Subsequently, since we do not have a DSD from the rain gauge, we hypothesize that it has the form of an exponential αeβ, and we interpolate these parameters from the disdrometer data. Then this parametrs are used to apply corrections to nearby rain gauge measurements, and the corrected and uncorrected values are compared. These differences are found to be statistically significant. Furthermore, twenty-six stations in Calabria, equipped with rain gauges and anemometers, are analyzed using the same DSD parameters derived from the Pescara dataset. Precipitation amounts obtained from corrected and uncorrected DSDs are compared with corresponding corrected and uncorrected rain gauge data, revealing statistically significant differences. These findings provide insight into the effects of the applied correction on rain rate measurements.
Acknowledgments
This work was carried out within the framework of the ongoing Italian national project PRIN2022MYTKP4 “Fostering innovation in precipitation measurements: from drop size to hydrological and climatic scales”.

How to cite: Adirosi, E., Parasporo, L., Baldini, L., Cauretuccio, A., Chinchella, E., Caloiero, T., and Lanza, L.: The wind effects on disdrometer and rain gauges measurements: results from a 4-year long rain series data-set in Pescara and a 10-year long rain series data-set in Calabria (Italy), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15409, https://doi.org/10.5194/egusphere-egu25-15409, 2025.

EGU25-15697 | ECS | PICO | HS7.1

Rain scintillation spectra from microwave links: A potential source of information for raindrop size distributions 

Peiyuan Wang, Arjan Droste, Marc Schleiss, and Remko Uijlenhoet

Rainfall has been monitored with microwave links opportunistically for nearly 20 years. So far, most studies have focused on retrieving rainfall rates using the mean received signal, based on the power-law relation between specific attenuation and rainfall rate. However, theories and measurements have indicated that the power spectral density (PSD) of received signal contains extra information about rainfall. The drop size distribution (DSD) and the motion of raindrops both play a role in determining the scintillation spectrum of rain. To evaluate the feasibility of making use of rain spectra for retrieving information about DSDs, measurements from different experimental datasets are investigated. Initial results indicate that some information about rainfall (e.g. rainfall rate) is indeed retained in the spectra measured by a radio link at 26 GHz and a scintillometer at 160 GHz. Furthermore, a simulation of the PSD of the received voltage during rain is made to gain understandings of its behavior. The simulation, based on Ishimaru’s work (1978), allows for the customization of various settings (e.g., wavelength, geometry, antenna gain functions) of radio links, as well as the DSD at different locations along the links. It is shown that large raindrops have more influence on the PSD of received voltage than smaller raindrops. A theoretical method to retrieve DSD from the PSD of the received voltage is proposed and its performance is assessed by simulation. Results show that the concentration of the tiniest raindrops is hard to retrieve because of their minor impacts on PSD. In the simulation, the concentration of larger raindrops can be relatively reliably retrieved, even when a large variation of DSDs is present along the microwave link.

How to cite: Wang, P., Droste, A., Schleiss, M., and Uijlenhoet, R.: Rain scintillation spectra from microwave links: A potential source of information for raindrop size distributions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15697, https://doi.org/10.5194/egusphere-egu25-15697, 2025.

EGU25-15743 | ECS | PICO | HS7.1

Small-scale spatial rainfall variability during the extreme convective rain event of June 11th, 2018, over the city of Lausanne 

Adrien Liernur, Lionel Peyraud, Marco Gabella, Urs Germann, and Alexis Berne

Localized and Intense Rainfall Events (LIREs) can cause significant societal and economic damages. Typically developing over very small spatial and temporal scales, the accurate characterization and forecasting of such events remains, however, particularly challenging. By collecting distributed space-time observations, weather radars can provide useful information for the analysis of such events. In this study we take advantage of the experimental high-resolution radar data from the MeteoSwiss operational radar network available at 83 m radial resolution, every 5 minutes, over 20 different elevations to analyze the small-scale spatial variability associated with the extreme Lausanne LIRE of June 11th, 2018, leading to the largest ever recorded 10-min rain gauge accumulation in Switzerland (41 mm). First, investigating the large-scale processes associated with this extreme event, a synoptic and dynamic analysis was conducted. This revealed the presence of a moderately unstable maritime tropical airmass which aided in the formation of a multicell thunderstorm which produced a wet microburst right over the city of Lausanne pouring an enormous quantity of water over very small spatial and temporal scales and leading to considerable localized flood and wind damage. Then, relying on the high-resolution radar data, the variability at small scale was measured by comparing rain rate values derived at different resolutions. More specifically, starting from the 83 m radar data, different existing hydrometeor-specific Z-R / Z-S relationships were used to compute an equivalent rain rate value at the gate level. Those were then compared against the corresponding rain rate values integrated at coarser radial resolutions of 500 m and 1000 m, and the difference across resolutions was derived as an indicator of small-scale spatial variability. With 1.5%, 0.41% and 0.18% of the total extracted and pre-processed gate volume showing differences larger than 25, 50 and 75 mm/hr between the 83 m and the 500 m data, a few but extreme small-scale rainfall variability peaks were observed, mostly associated with intensity peaks. Although most of these peaks were located above or within the melting layer, several of them were still observed below the melting layer, at proximity to the ground, and potentially decisive for hydrological applications. Converting this 3D information into 2D maps of sub-grid variability, a significant variability at the 5 min / 1km2 resolution was observed highlighting not only the highly dynamic evolution of this event but also and the added value of high-resolution radar data to capture small-scale peaks associated with this extreme LIRE. By providing complementary insights on rainfall variability peaks, the retrieved sub-grid information can help improve the characterization of LIRE and enrich existing rainfall products.

How to cite: Liernur, A., Peyraud, L., Gabella, M., Germann, U., and Berne, A.: Small-scale spatial rainfall variability during the extreme convective rain event of June 11th, 2018, over the city of Lausanne, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15743, https://doi.org/10.5194/egusphere-egu25-15743, 2025.

EGU25-17651 | PICO | HS7.1

Wind tunnel experiments to evaluate the wind-induced bias on disdrometer measurements 

Luca G. Lanza, Enrico Chinchella, Filippo Calamelli, Arianna Cauteruccio, and Daniele Rocchi

Wind has a significant impact on precipitation measurement instruments, including disdrometers, by inducing aerodynamic disturbances around their bodies. These airflow features divert trajectories of falling hydrometeors, often reducing the amount of precipitation detected when compared to  windless conditions. Furthermore, the shape of disdrometers, which is non-radially symmetric, makes the wind-induced bias dependent on wind direction. Traditionally, field experiments have been used to develop corrections for the wind-induced bias. However, Computational Fluid Dynamics (CFD) simulations offer a more versatile approach for studying wind-induced bias on different instrument designs under varying climatic conditions. In this work a wind tunnel experimental campaign was conducted to show the interaction between wind and disdrometers and to validate a suitable CFD model by providing detailed data on drop trajectories. Full-scale tests were conducted in the high-speed test section of the Wind Tunnel facility available at Politecnico di Milano. The chamber (4m wide, 3.8m high and 6m long) is characterized by a nearly laminar flow and a narrow boundary layer. The disdrometers were fixed to the ground on a rotating plate to facilitate alignment with the flow direction. Furthermore, a specially designed drop generator – attached to a moving gantry – was used to release water drops into the wind flow, allowing precise control of drop diameter, release height and timing. Finally, a high-speed camera, operating at 1000 fps, recorded the trajectories of the drops approaching the sensing areas of the disdrometers. Images were processed to identify each drop, calculate their velocity and track their movement through the camera field of view. The study focused on two disdrometer models, the Thies CLIMA LPM and the OTT Parsivel2, which use an optical method to measure drop size and velocity. The experiments were conducted for wind speeds of 10 m/s, drop diameters ranging from 1.0 to 1.2 mm, and three wind directions (0°, 45°, and 90°). Results showed that wind significantly alters drop trajectories, often diverting them away from the sensing area or causing them to collide with the instrument body. A numerical model - already used in e.g., Chinchella et al., (2024) – was validated by simulating the experimental conditions and comparing the results against observations. Validation shows that the numerical approach is suitable for developing adjustment curves to correct disdrometer measurements under windy conditions. This work further highlights the importance of addressing wind effects in precipitation measurements, by applying correction curves (see e.g., Chinchella et al., 2024) to enhance the accuracy of rainfall measurements obtained from disdrometers like the Thies CLIMA LPM or the OTT Parsivel2.

ACKNOWLEDGMENTS

The wind tunnel campaign on disdrometers was carried out within the framework of the Italian national projects PRIN2022MYTKP4 “Fostering innovation in precipitation measurements: from drop size to hydrological and climatic scales”.

References:

Chinchella E., Cauteruccio, A., & Lanza, L. G. (2024). Quantifying the wind-induced bias of rainfall measurements for the Thies CLIMA optical disdrometer. Water Resources Research, 60(10), e2024WR037366. https://doi.org/10.1029/2024WR037366   

How to cite: Lanza, L. G., Chinchella, E., Calamelli, F., Cauteruccio, A., and Rocchi, D.: Wind tunnel experiments to evaluate the wind-induced bias on disdrometer measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17651, https://doi.org/10.5194/egusphere-egu25-17651, 2025.

EGU25-17854 | PICO | HS7.1

Assessing the Impact of Weather Conditions on Radar-Based Rainfall Estimation in the Tropics: A Case Study in Thailand 

Narongrit Luangdilok, Ruben Imhoff, Claudia Brauer, and Albrecht Weerts

In hydrological modeling and forecasting, rainfall data is a key factor in determining the model’s accuracy. The higher the accuracy of the estimated rainfall, the more accurate the model’s predictions can be. Rain gauges can be utilized to estimate the amount of rainfall within a catchment area but their effectiveness is often limited by the sparse distribution of rain gauges and the lack of sufficient spatial information they provide for comprehensive distributed hydrological simulations. Weather radar serves as an alternative source of rainfall data, capable of providing remotely sensed rainfall estimates with high temporal and spatial resolution. However, conventional radar quantitative precipitation estimation (QPE) is subject to uncertainties, primarily arising from variations in the drop size distribution (DSD) of hydrometeors and variations in vertical profile reflectivity (VPR). Those variations are typically influenced by the local climate and weather conditions and their impacts on the performance of QPE remains a subject of research especially in tropical regions. Therefore, this study aims to investigate relationships between weather conditions and the performance of radar QPE using statistical and machine learning approaches at different time scales. In Thailand, the radar-based rainfall data is derived with a standard fixed power law relationship between radar reflectivity and rain rate, from three weather radars located in different parts of the country. The rainfall estimates from this radar rainfall product are investigated with weather conditions from ERA5 reanalysis datasets and local observations in the period of 2022-2024. The findings help us to identify the key factors influencing the accuracy of radar rainfall estimation, which can be used to improve radar rainfall estimation, for example through finding adequate predictors for the construction of a dynamic Z-R relationship in tropical conditions. Future studies could expand this analysis by integrating these impact factors into radar QPEs and implementing improved estimated rainfall products in hydrological models.

How to cite: Luangdilok, N., Imhoff, R., Brauer, C., and Weerts, A.: Assessing the Impact of Weather Conditions on Radar-Based Rainfall Estimation in the Tropics: A Case Study in Thailand, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17854, https://doi.org/10.5194/egusphere-egu25-17854, 2025.

EGU25-3598 | ECS | Orals | GM2.7

An extended CFD-DEM model based on micropolar fluid for debris flow 

Lian Wang, Xihua Chu, and Hongguang Sun

CFD (computational fluid dynamics)-DEM (discrete element method) model has been widely applied in the simulation of the multiphase flow involving granular materials, but it’s time-consuming for the calculation of a large number of particles with different sizes in DEM. In this study, a model based on the computational micropolar fluid dynamics and discrete element method, viz. a CMFD-DEM model, is proposed to describe the coupling system that consists of gas-liquid two phases and discrete particles with different sizes. In this model, micropolar fluid model is employed to describe the mixture of the pure fluid with fine particles, while discrete element method is used to calculate the motion of the larger particles. In addition, VOF (volume of fluid) method is adopted to track the free surface of the liquid. The implementation of the CMFD-DEM model is based on the open source software, OpenFOAM and LIGGGHTS, and is validated in single particle sedimentation and particles pouring into quiescent water cases. Then, the simulation of debris flow is carried out. The results show that specific dynamic behaviors of debris flow can be reproduced by CMFD-DEM model. The average velocity and runout of debris flow are decreased with the increase of micropolar parameter N/L. Through the comparisons to the exiting results, it suggests that CMFD-DEM model is capable to describe the multi-size effect of the granular materials in debris flow.

How to cite: Wang, L., Chu, X., and Sun, H.: An extended CFD-DEM model based on micropolar fluid for debris flow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3598, https://doi.org/10.5194/egusphere-egu25-3598, 2025.

Transport of granular materials on Earth and planetary surfaces are at the heart of landscape dynamics and geohazards. These transport phenomena are controlled by particle-scale mechanisms, including particle motion, collisions, and interactions with the ambient fluid, which highlights the importance of particle-resolved measurements in physical experiments. However, despite recent progress in particle tracking velocimetry (PTV) for spherical (and regularly shaped) particles, there still lacks a robust technique in tracking and analyzing the motion of non-spherical particles, particularly because conventional PTV cannot identify moving objects of an arbitrary shape. This limitation largely compromises our particle-scale understanding of the transport of natural granular materials with a wide range of shapes and sizes. To tackle this issue, we propose a novel deep learning-based PTV framework for arbitrarily shaped and sized particles, which consists of a real-time computer vision algorithm called YOLO (you only look once) and an accurate inter-frame matching algorithm based on Kalman filtering. The proposed PTV framework is validated in various granular flow and sediment transport scenarios, using high-resolution data obtained from discrete element method simulations and small-scale physical experiments. Using this new technique, we are able to precisely analyze the kinematics information of spherical, non-spherical, and mixed particles with different concentrations in a series of open channel bedload transport experiments. Scaling relations are obtained between the sediment flux and bed shear stress to reveal the effects of particle shape and composition on the sediment transport dynamics across bedload and sheet flow conditions. The proposed PTV technique and its potential applications are expected to provide a new avenue for future research on the micromechanical aspects of geophysical granular flow and sediment transport.

How to cite: Su, W., Jing, L., and Xu, M.: Deep learning-based particle tracking velocimetry (PTV) for spherical and non-spherical particles: Application to granular flow and sediment transport, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7708, https://doi.org/10.5194/egusphere-egu25-7708, 2025.

Step-pools are common bedforms in mountain streams and have been utilized in river restoration or fish passage projects around the world. Step-pool units exhibit highly non-uniform hydraulic characteristics which have been reported to closely interact with the morphological evolution. Further understanding towards these interactions builds the basis for better prediction of channel evolution and more advanced design of artificial step-pool system. However, detailed information on the flow-morphology interactions has been limited due to the difficulty in measuring the flow structures or the flow forces in a step-pool unit.

To fill in this knowledge gap, we established an approach combining physical experiment and computational fluid dynamics (CFD) simulation for a step-pool unit made of natural grains at six flow conditions. Structure from motion (SfM) was used to capture the detailed 3D reconstructions of the bed surfaces with various conditions of pool scour. The hydraulic measurement was applied both as input data at the inlet boundary and also in the validation for the CFD model. The high-resolution 3D flow structures for the step-pool unit were visualized, as well as the distributions of flow forces from both pressure and shear stress.

The results illustrate the segmentation of flow velocity downstream of the step, i.e., the integral recirculation cell at the water surface, streamwise vortices formed at the step toe, and high-speed flow in between, resulting from the complex morphology of the step-pool unit. Both the recirculation cells at the water surface and the step toe perform as energy dissipaters to the flow with comparable magnitudes. Pool scour development during flow increase leads to the expansion of the recirculation cells until step-pool failure occurs. Significant transverse variability of the flow forces from both the shear stress and pressure has been revealed. The flow forces in both streamwise and transverse directions are closely related to the flow structures and morphology in the unit. The ratios between skin and form drag have large variations at low flows while show a relatively limited range of 0.05-0.1 at high flows, suggesting a small proportion occupied by the skin resistance in the total flow resistance in the step-pool channel. The drag coefficient of the step-pool unit is around 0.3 at high flows. Our results highlight the feasibility of the approach combining physical and numerical modeling in investigating the complex flow-morphology interactions of step-pool features.

How to cite: Zhang, C., Hassan, M., and Xu, Y.: Investigating interactions between flow and morphology in a step-pool unit combining physical and numerical modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7900, https://doi.org/10.5194/egusphere-egu25-7900, 2025.

EGU25-7958 | ECS | Posters on site | GM2.7

Finite-Size Effects in Geophysical Granular Flow from a Nonlocal Rheology Perspective 

Jiacheng Xia, Lu Jing, and Ming Peng

Geophysical granular flow is ubiquitous in nature and plays a crucial role in shaping the landscape (hillslope creep, riverbed evolution) and causing geohazards (landslide, debris flow). Small-scale models are an effective way to understand these natural phenomena at large scales. However, finite-size effects inevitably occur due to the multi-scale nature of granular materials, hindering integration of mechanisms obtained from small-scale investigations and continuum models (e.g., granular flow rheology) for large-scale applications. Here we use granular column collapse as a model case to address finite-size effects in granular flows from a novel rheological perspective. We computationally simulate column collapse of varying system-to-particle size ratios using the discrete element method and extract detailed local rheological information during the flow via a coarse-graining technique. We find a disproportional increase in the dimensionless runout distance with the system-to-grain size ratio and a significant difference in the dynamic process. This discrepancy is reflected in the μ(I) curve as non-collapsed data at low inertial number regimes, but casting the data into a non-local rheology framework proposed by Kim and Kamrin (2020) leads to data collapse onto a single master curve for all simulations. This indicates that the finite-size effect is controlled by velocity fluctuations at the grain scale and is a manifestation of the non-locality of granular materials. As a result, the introduction of an intermediate length scale that reflects velocity fluctuations is expected to enable accurate modeling of geophysical granular flows with varying system and particle sizes in a unified continuum framework. It also provides a new perspective for continuum modeling of polydispersity, size segregation, hysteresis, and other size-dependent phenomena in geophysical granular systems.

How to cite: Xia, J., Jing, L., and Peng, M.: Finite-Size Effects in Geophysical Granular Flow from a Nonlocal Rheology Perspective, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7958, https://doi.org/10.5194/egusphere-egu25-7958, 2025.

EGU25-8700 | Posters on site | GM2.7

Quantification of intense transport of fractions of stratified bimodal bed load based on measured distributions of velocity and concentration 

Vaclav Matousek, Jan Krupicka, Tomas Picek, and Lukas Svoboda

We present the results of laboratory experiments investigating the intense transport of bimodal bed load under high bed shear conditions in a tilting flume. Particles of two lightweight sediment fractions, differing in size, tend to separate during transport above the plane surface of an eroded mobile bed. Coarser fraction particles are predominantly present in the collisional layer above the bed, while finer fraction particles are primarily concentrated in the interfacial layer, which develops between the eroded bed and the collisional layer. This observed stratification of transported fractions influences their respective contributions to the total bed load discharge through the flume. Vertical distributions of local velocity and volumetric concentration were measured across the flow depth for each fraction separately, allowing the determination of each fraction's proportion in the total discharge. The experimental results were combined with a previously collected dataset to compare the discharges of bimodal and unimodal sediments under hydraulically similar conditions. Additionally, the experimentally determined discharges were evaluated against predictions from transport models designed for intense unimodal and bimodal bed loads.

How to cite: Matousek, V., Krupicka, J., Picek, T., and Svoboda, L.: Quantification of intense transport of fractions of stratified bimodal bed load based on measured distributions of velocity and concentration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8700, https://doi.org/10.5194/egusphere-egu25-8700, 2025.

EGU25-8745 | ECS | Posters on site | GM2.7

Reliability-Based Analysis of Initiation of Sediment Motion on Movable Bed 

Selman Baysal, V. Ş. Özgür Kırca, and Manousos Valyrakis

Sediment transport dynamics are of great importance in understanding geophysical flows, where determining the threshold conditions for the initiation of sediment motion presents a complex challenge. In a pioneering work, Shields (1936) established the Shields’ criterion to assess the critical shear stress (τc) required for sediment motion in non-turbulent flows. Although this approach has significant advantages, including a robust empirical foundation and the implementation of non-dimensional critical shear stress, it is valid for limited conditions since it oversimplifies vital aspects such as sediment heterogeneity and complex flow interactions.

In turbulent flows, the effective critical shear stress acting on a grain may become higher than that measured in the case of laminar flows (i.e., the average critical stress, τc, defined by Shields, 1936) as a result of fluctuations in the shear stress (τ′). Owing to this, in geophysical turbulent flows near the threshold of motion, neither the driving nor the resisting parameters of sediment motion have crisp values; instead, they may be considered probabilistic parameters. The reliability-based approach is applied here in to handle the complex nature of the initiation of sediment motion.

This study aims to present preliminary results of research that aims to enhance the knowledge of incipient motion by applying a reliability-based analysis of Shields’ criterion based on the theory and empirical equations adopted by Zanke (2003). In this analysis, the turbulence parameter (n) and angle of repose (ϕ) are introduced as key parameters regarding the initiation of sediment motion. These parameters are generated as random variables by means of Monte Carlo Simulations, introducing various probabilistic distributions (e.g., normal, log-normal, triangular, gamma) and statistical moments (e.g., mean, standard deviation).

By simulating a wide range of angles of repose and turbulence parameters with Monte Carlo Simulations, the inherent uncertainties in sediment transport and the complexity of hydrodynamic models are incorporated. In this work critical shear stresses of thousands of grains are assessed for different grain Reynolds numbers. As a result, threshold of motion curves are probabilistically derived, indicating confidence for grain entrainment, and establishing a model that enables risk assessment and decision-making for a wide range of scenarios. Comparisons of model results with empirical data show that the model captures the complex physical process.

How to cite: Baysal, S., Kırca, V. Ş. Ö., and Valyrakis, M.: Reliability-Based Analysis of Initiation of Sediment Motion on Movable Bed, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8745, https://doi.org/10.5194/egusphere-egu25-8745, 2025.

Avalanches of dry granular materials, such as rocks, snow, and ice, are chief contributors to hazardous geophysical flows in nature. A key problem hampering progress in predicting the destructiveness of such hazards is the poorly understood dependence of the flow velocity on the physical properties of the grains constituting a given material. In particular, their usually irregular, non-spherical shapes prevent application of rigorous theories, which were derived for spherical grains. In addition, we do not have a good empirical grasp of the issue, as evidenced by the failure of existing scaling laws across flows of different granular materials when applied to measurements and numerical simulations for idealized flow geometries. Here, we report a scaling law for the steady-state velocity of homogeneous granular flows down rough inclines. It holds for granular materials consisting of irregularly-shaped but relatively uniformly-sized grains descending rough slopes. Laboratory chute experiments and numerical simulations for a diverse range of granular materials corroborate its validity and generality. It exhibits a power-4/3 dependence on the flow thickness, as opposed to the power-3/2 dependence suggested by previous scaling laws. It is also unique in the aspect that it depends only on a single parameter characterizing the granular material: the dynamic angle of repose. This suggests that, quite surprisingly, most of the physical complexity associated with the composition and shape of a material's grains boils down to its bulk ability to resist externally-driven shearing.

How to cite: Pähtz, T.: General scaling law for the velocity of steady, homogeneous granular flows down rough inclines, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9678, https://doi.org/10.5194/egusphere-egu25-9678, 2025.

EGU25-9842 | ECS | Orals | GM2.7

Turbulence increases sediment transport 

Daniel Rebai, Katinka Koll, Alessio Radice, Jochen Aberle, and Francesco Ballio

In steady, fully developed flows over erodible beds, the average bed shear stress is generally the dominant factor governing sediment flowrate. However, fluctuations induced by turbulence can play a significant role in altering sediment transport dynamics. This study investigates the effects of such turbulence by conducting flume experiments with flow disturbances created by various cylinder arrays placed in the flow. To measure the turbulent flow field, Laser Doppler Velocimetry (LDV) was employed, while bed shear stress was quantified using a shear plate. The bedload motion was analysed using Particle Tracking Velocimetry (PTV), which allowed for the quantification of key variables such as sediment concentration, velocity, and sediment flowrate. A descriptive model was developed to capture the relationship between these primary variables and both the average and fluctuating components of the flow. Our results show that with increasing turbulent fluctuations, both sediment concentration and velocity rise at a fixed mean shear stress. Notably, turbulence influences concentration more strongly than velocity.

How to cite: Rebai, D., Koll, K., Radice, A., Aberle, J., and Ballio, F.: Turbulence increases sediment transport, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9842, https://doi.org/10.5194/egusphere-egu25-9842, 2025.

EGU25-10237 | Orals | GM2.7

Unified flow rule of undeveloped and fully-developed dense granular flows down rough inclines 

Yanbin Wu, Thomas Pähtz, Zixiao Guo, Lu Jing, Zhiguo He, and Jinchuan Zhang

We report on chute measurements of the free-surface velocity $v$ in dense flows of spheres and diverse sands and spheres-sand mixtures down rough inclines. These and previous measurements are inconsistent with standard flow rules, in which the Froude number $v/\sqrt{gh}$ scales linearly with $h/h_s$ or $(\tan\theta/\mu_r)^2h/h_s$, where $\mu_r$ is the dynamic friction coefficient, $h$ the flow thickness, and $h_s(\theta)$ its smallest value that permits a steady, uniform dense flow state at a given inclination angle $\theta$. This is because the characteristic length $L$ a flow needs to fully develop can exceed the chute or travel length $l$ and because neither rule is universal for fully-developed flows across granular materials. We use a dimensional analysis motivated by a recent unification of sediment transport to derive a flow rule that solves both problems in accordance with our and previous measurements: $v=v_\infty[1-\exp(-l/L)]^{1/2}$, with $v_\infty\propto\mu_r^{3/2}\left[(\tan\theta-\mu_r)h\right]^{4/3}$ and $L\propto\mu_r^3\left[(\tan\theta-\mu_r)h\right]^{5/3}h$.

How to cite: Wu, Y., Pähtz, T., Guo, Z., Jing, L., He, Z., and Zhang, J.: Unified flow rule of undeveloped and fully-developed dense granular flows down rough inclines, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10237, https://doi.org/10.5194/egusphere-egu25-10237, 2025.

Progressive slope steepening can trigger episodic dry sand avalanches, resembling landslides commonly observed in natural environments. Similarly, gradual river incision can induce periodic slope instability and failures. To thoroughly investigate the impact of gradual river incision on catchment topography and slope dynamics, we conduct a series of idealized dry sandbox experiments. This simple setup is expected to provide a deeper understanding of the patterns and dynamics of landslides in mountainous regions.

In the experiments, dry sand is removed by applying negative suction pressure through a nozzle traversing prescribed paths over the topography. This process simulates river channel incision into the sand substrate and triggers avalanches on adjacent slopes. The experimental setup consists of a simple box filled with dry sand, equipped with a suction mechanism inspired by the extrusion nozzles used in 3D printing. Unlike 3D printing, where material is added, negative pressure at the nozzle is used to extract material instead.

To validate the system, we first employ a vertically descending suction nozzle at a controlled rate to produce an expanding conical pit. This simple setup allows us to test the suction mechanism and ensure consistent material removal. Subsequently, we simulate river incision by utilizing an idealized curved path designed to mimic the geometry of an incising river. Initially, the nozzle was manually guided along this path to replicate the incision process. In later experiments, a computer-controlled traversing system is implemented to ensure greater precision and reproducibility.

We then explore imposed motions along the main river channel and incorporate tributaries to explore the river incision processes. The results, including the formation of ridges, avalanches, and slope adjustments, are analyzed and compared with computational predictions derived from an eikonal model. This comparison provides valuable insights into the behavior of slopes under conditions of gradual river incision and elucidates the mechanisms driving slope instability and morphological evolution in natural catchments.

How to cite: Chang, E. and Capart, H.: Experimental Analogue Modeling of Slope Dynamics Induced by Gradual River Incision Using a Controlled Suction Nozzle in Dry Sandbox Experiments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12716, https://doi.org/10.5194/egusphere-egu25-12716, 2025.

EGU25-13548 | Posters on site | GM2.7

Shallow-water continuum modelling of dry granular flows in partailly obstructed chutes  

Rui Miguel Ferreira and Solange Mendes

We employ data about a dry granular flow down a 19º smooth-walled chute, partially obstructed at the downstream end, to verify the solution of a shallow-water continuum model. The system of conservation equations is based on depth-averaging the ensemble-averaged mass, momentum and fluctuating kinetic energy equations:

(1)  $\partial_t \left(\phi h \right) + \partial_x \left(\phi h u \right) = - \partial_t z_b$

(2)  $\partial_t \left( \rho h u \right) + \partial_{x} \left( \rho h u^2 \right)  = -\partial_{x} \left( \rho g h^2 / 2 \right) - g \rho h \, \partial_{x} z_b  - \tau_b$

(3) $\partial_{t} z_b = - \left( E(x,t) - D(x,t) \right)$

(4) $P = f(\phi) f(e,k,\phi_c) \rho_g T$

(5) $-Q^\prime + \frac{1}{2}\tau_b u/h - \Gamma = 0$

where $x$ is the distance, $t$ is time, the conservative variables are the elevation of the granular bed, $z_b$, the equivalent depth of flowing granular material $\phi h$ and flow momentum $\rho \phi h$, where $\phi$ is the solid fraction, $h$ the granular depth and $u$ the depth-averaged longitudinal velocity, $\tau_b$ is the wall stress, $E$ and $D$ are the rates of particle pick-up and deposition, respectively, $e$ is the normal coefficient of restitution, $k$ is particle stiffness, $\phi_c$ is the critical solid fraction, $\rho_g$ is the density of the solid particles, $\rho = \rho_g \phi$, $\Gamma$ is the rate of dissipation of fluctuating kinetic energy and $Q^\prime$ is the flux of fluctuating kinetic energy at the bottom wall.  The solid fraction is determined from (4) as a function of the granular pressure $P$ (considered hydrostatic) and the granular temperature $T$.

Preliminary results of simulations with borosilicate spheres ( g/cm3 and coefficient of restitution ), with  and  as tuning parameters, indicate that the celerity of the jamming wavefront is well-reproduced. The jump strength and the head losses are not in full agreement, requiring adjustments in the equation of state (4).

 

Acknowledgements

Portuguese Foundation for Science and Technology (FCT) through the PhD scholarship PD/BD/150693/2020, project PTDC/ECI- EGC/7739/2020 and CERIS funding UIDB/04625/2020.

How to cite: Ferreira, R. M. and Mendes, S.: Shallow-water continuum modelling of dry granular flows in partailly obstructed chutes , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13548, https://doi.org/10.5194/egusphere-egu25-13548, 2025.

EGU25-13625 | Orals | GM2.7

Formation and evolution of sediment ribbons in open-channel flow 

Olivier Eiff and Michele Trevisson

The formation and evolution of sediment ribons over a uniform sediment bed in an open-channel flow was investigated via a stereo-photogrammetric system to measure the bed evolution in combination with a stereo-PIV system to measure the three-component velocity field in a cross-sectional plane above the bed. The formation of ribbons is observed to be triggered by the initially meandering low and high-speed streaks sharing the same spanwise wavelength as the fully-developed ribbons.  When the ribbons are fully developed, the streaks are locked in place with low-speed streaks over the ridges and high-speed streaks over the troughs with strong secondary flows.  The lateral stabilization appears to be facilitated by the stable  streaks near the wall.

How to cite: Eiff, O. and Trevisson, M.: Formation and evolution of sediment ribbons in open-channel flow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13625, https://doi.org/10.5194/egusphere-egu25-13625, 2025.

EGU25-14061 | ECS | Posters on site | GM2.7

Experimental investigation on the formation and failure of landslide dam using inertial navigation method 

Ran Li, Yi-ming Li, Tong-Tong Mu, and Hong-yang Dai

Landslides in narrow valleys may block adjacent rivers and dam the incoming water flow. The collapse of these landslide dams may lead to catastrophic flooding downstream. The measurement and early warning of dam failures is an important issue in geomorphic processes. However, Optical and radar-based monitoring methods are not suitable for deep internal probing of a dam, which is necessary for dynamic measurement and early warning. In this study, the acceleration of a smart rock in the simulation dam was measured using inertial navigation method. It is found the acceleration response of smart rocks is detected more than 20 seconds before external observations of dam failure. Buried at different positions within a dam, smart rocks exhibit distinct temporal and data form responses to dam failure. Smart rocks located deeper within the dam show multiple acceleration fluctuations before the actual failure occurs. We hope that the measurement data provided by smart rocks will assist in developing multi-scale models of dam failure.

How to cite: Li, R., Li, Y., Mu, T.-T., and Dai, H.: Experimental investigation on the formation and failure of landslide dam using inertial navigation method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14061, https://doi.org/10.5194/egusphere-egu25-14061, 2025.

EGU25-14133 | Orals | GM2.7

Energetic kinetic of debris flow in a horizontal chute using centroid vector displacement method 

Hui Yang, Zhipeng Chi, Quan Chen, and Yue Xu

Debris flows, as a type of large-scale geological disaster, are a global focus regarding their formation boundary, kinematic properties and deposit morphology. In small-scale laboratory simulations, factors such as water content, equivalent grain size, grain size ratio and aspect ratio significantly influence the formation boundaries and flow regime. Quantifying the effects of these numerous variables is a crucial prerequisite for advancing research on geological disasters represented by debris flows. We conducted simulations of the debris flow triggering process within a horizontal chute and used the proposed centroid vector displacement method to quantitatively assess the kinetic characteristics from an energetic perspective. By integrating the influence of water content into the traditional Bond number, we were able to clearly differentiate three distinct collapse regimes. Through modulation of the size and density ratios, we explored the distribution of intensity for various mechanisms along the flow direction. To characterize the relative strength of diffusion and buoyancy effects on the length scale, we introduced a dimensionless parameter λ. This parameter enabled us to define the boundary conditions necessary for the formation of core-band patterns.

How to cite: Yang, H., Chi, Z., Chen, Q., and Xu, Y.: Energetic kinetic of debris flow in a horizontal chute using centroid vector displacement method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14133, https://doi.org/10.5194/egusphere-egu25-14133, 2025.

Alluvial fans develop at the base of mountain fronts, where rivers emerge from the constrained mountain area onto the plain. Acting as a transition zone between mountain streams and alluvial rivers, the fan-river system is typically characterized by a slope break in the bed profile, a significant discontinuity in bed surface sediment fining from gravel-sized to sand-sized, and a sudden increase in channel width. In large rivers with great morphological diversity and strong human interference, the shift between upstream and downstream river morphology and sediment dynamics within the alluvial fan-river system exhibits a more complex process. However, this phenomenon remains insufficiently documented and lacks comprehensive analysis.

Here, we take the middle Yangtze alluvial fan as an example and use field observations and numerical modeling to improve the understanding of the large-scale alluvial fan-river system. The result shows that, in contrast to other alluvial fan-river systems, the Yangtze alluvial fan downstream of the Three Gorges Valley had no obvious breaks in the recent bed profile. In addition, the channel width showed an abrupt increase at Zhicheng, followed by a narrowing trend beginning at Chenjiawan. After the Three Gorges Dam (TGD) operation in 2003, the erosive water released from the TGD induced significant erosion, however, the spatial pattern of the bankful width remained stable. The bed profile exhibited increasing variability but continued to lack a distinct slope break; The transition in surface material from gravel to sand was observed throughout approximately 60 kilometers and the location migrated 40 kilometers downstream in the post-TGD period, with gravel and sand patches alternating randomly; Zhicheng and Chenjiawan are two characteristic locations marking the shifts in the mode of sediment transport in the middle Yangtze alluvial fan-river system. For sand transport mode, the reach upstream of Zhicheng had sand transported in suspension, whereas the downstream reaches were dominated by mixed-load transport. For gravel transport mode, gravel from upstream, mostly in the 25–50 mm grain size range, was selectively transported downstream of Zhicheng and deposited at Chenjiawan; The sediment dynamics in the Yangtze alluvial fan-river system were controlled by the width variability and distributary streams. The deposition of fine sand upstream of the gravel smoothed the previously deposited gravel fan profile, resulting in the absence of a slope break in the bed profile. Since 2003, the pattern of the sediment transport mode remained stable despite some local adjustments. This stability is attributed to the stable fan-river morphology induced by the strong resistance of riverbank lithologies and the Jingjiang Great Levee constraints.

How to cite: He, Z., Sun, Z., Li, Y., Luan, H., and Qu, G.: Large-scale alluvial fan-river system of the middle Yangtze River: morphological diversity, grain size discontinuity, and sediment dynamics complexity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14540, https://doi.org/10.5194/egusphere-egu25-14540, 2025.

EGU25-14717 | Posters on site | GM2.7

Modeling Debris Flow Transitions: Experimental Validation and Field-Scale Application 

Chieh-Ya Liao, Yi-Ling Tsai, and Chi-Yao Hung

Debris flows, prevalent in mountainous regions, exhibit distinct dynamics depending on whether they occur over bedrock (rigid bed) or accumulated deposition (erodible bed). Understanding the transition between these bed types is essential for hazard prediction and mitigation. This study improves an existing unsteady, non-uniform debris flow model to more accurately simulate the evolution of flow depth and velocity under varying boundary conditions. The improved model is grounded in mass, momentum, and kinetic energy conservation principles, incorporating a linearized μ(I) rheology to describe granular flow behavior and Coulomb friction along sidewalls, ensuring a realistic representation of debris flow mechanics.

To validate the improved model, granular dam break experiments were conducted in a narrow glass channel (3.5 m long, 0.04 m wide) with varying downstream deposit depths to establish different basal boundary conditions. High-speed camera footage and Particle Tracking Velocimetry (PTV) were employed to capture granular motion and generate velocity fields. The model exhibited good agreement with experimental results, accurately predicting the flow depth and velocity evolution during the transition between rigid and erodible beds.

Furthermore, the model was applied to field-scale debris flows at the PuTunPunas River in southern Taiwan, a site that has experienced several debris flow events over the past decades. Channel width variations at this site were incorporated into the model to assess erosion potential and flow behavior under real-world conditions. Comparisons with field observations confirmed the model’s capability to simulate debris flow transitions and erosion processes in natural channels, offering valuable insights for hazard assessment and mitigation in mountainous regions.

How to cite: Liao, C.-Y., Tsai, Y.-L., and Hung, C.-Y.: Modeling Debris Flow Transitions: Experimental Validation and Field-Scale Application, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14717, https://doi.org/10.5194/egusphere-egu25-14717, 2025.

EGU25-14812 | ECS | Orals | GM2.7

Slowflows: Experiments and numerical simulations 

Parameshwari Kattel, Chet N. Tiwari, and Shiva P. Pudasaini

Due to various destabilizing factors such as hydro-thermo-mechanical degradation, and earthquakes, the strength of the Earthsurface material may decrease, leading to increased slow earthflow events. Earthflows often cause extensive damage to infrastructure and permanently change the landscape pattern. However, the earthflows have received much less attention compared to their fast-moving counterparts, like avalanches, landslides, and debris flows. Here, we present some novel laboratory experiments simulating slowflows to understand their initiation, movement, and long-term morphological evolution by using a highly viscous material, the molten jaggery, locally found in Kathmandu. The tremendously slowly deforming and moving jaggery is assumed to represent earthflows. Experimental results demonstrate some key aspects of slowflow dynamics of earth materials and seminally contribute to the systematic understanding of earthflow processes. We simulate the slowflow propagation process by using a dynamic earthflow model. Simulation results capture some essential features of the massively viscous, exceptionally slowly deforming, and moving earth surface materials. 

How to cite: Kattel, P., Tiwari, C. N., and Pudasaini, S. P.: Slowflows: Experiments and numerical simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14812, https://doi.org/10.5194/egusphere-egu25-14812, 2025.

EGU25-15011 | ECS | Orals | GM2.7

Suspended Sediment Concentration Analysis Using Remote Sensing and Machine Learning Approach 

Srikanth Bhoopathi, Manali Pal, and Harshitha Choubey

This study employs remote sensing technology to thoroughly analyse sediment dynamics in expansive aquatic environments, with a specific focus on the Ganga River basin. The investigation spans from 2007 to 2011, utilizing Medium Resolution Imaging Spectrometer (MODIS) MYD09A1.061 Aqua Surface Reflectance 8-Day Global data to assess Suspended Sediment Concentration . By integrating ground-based silt data with satellite data, the study captures temporal variations in suspended sediment levels. The Google Earth Engine (GEE) platform was employed to process sensor imagery and calculate reflectance data, enabling accurate computations for specific time intervals. To further analyse the data, Support Vector Regression (SVR) model was developed. This model analyse changes in reflectance data  to corresponding  observed silt measurements, providing insights into sediment behavior. The results from this model are presented using 2D graphs, highlighting the  effectiveness of remote sensing technology in understanding the sediment dynamics in large river systems. This research offers significant advancements in  methods for monitoring and maintaining water quality in aquatic environments.

How to cite: Bhoopathi, S., Pal, M., and Choubey, H.: Suspended Sediment Concentration Analysis Using Remote Sensing and Machine Learning Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15011, https://doi.org/10.5194/egusphere-egu25-15011, 2025.

Sediment transport in turbulent flows is one of the classical topics in rivers and coastal engineering studies. Due to a lack of general description of interphase interactions, the numerical studies are limited by separately describing the motion of sediment particles in the form of bedload or suspended load depending on the relative importance of particle-particle and particle-turbulence interactions. In this paper, a Reynold-averaged Euler-Lagrange model is developed to study bedload and suspended load simultaneously where the interphase interactions are described in a unified mechanical framework. The inter-particle interactions are resolved and the flow turbulence is described by a modified two-phase k-epsilon turbulence model. Particle-fluid interactions at the volume-averaged scale are characterized by the drag force, the pressure gradient force and the lift force. The effects of the interstitial fluid on particle contacts are taken into consideration by formulations of coefficient of restitution and friction coefficient. A modified Continuous Random Walk (CRW) model is adopted to characterize the stochastic motion of the sediment particles. The effectiveness of the model in describing particle-turbulence and particle-particle interactions is firstly demonstrated by comparison with experiments of sediment transport in bedload and suspended load separately. The model is further applied to the study of sediment transport in sheet flows. Contributions of particle-turbulence and particle-particle interactions to the flow structure, the total transport rate and the rheology of particle-fluid mixtures are analyzed.

How to cite: Li, W.: A general description of interphase interactions in Reynolds-averaged Euler-Lagrange simulations of turbulent sediment transport: from bedload to suspended load, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15155, https://doi.org/10.5194/egusphere-egu25-15155, 2025.

Bedload transport, critical in various natural and engineering systems, involves the complex interaction between particles and flowing water. Predicting bedload transport rates has long been a focal point of interest due to its significance in understanding river dynamics. Pioneering contributions from Einstein and Bagnold have led to substantial progress in this field derived from extensive laboratory and in-situ observations, which are yet to achieve the desired accuracy when validated against real-world hydrological data. The discrepancies in predictions can partly be attributed to the difficulties in accurately capturing the movements of near-bed particles and the flow field characteristics.

This paper presents a numerical investigation via Computational Fluid Dynamics-Discrete Element Method into detailed observations on particle movements and flow characteristics of bedload transport. It provides a thorough review of the assumptions and theories prevalent in current bedload models. Simulations have been conducted covering flow velocities ranging from below the generally accepted critical Shields number to the onset of bedform formation. We analyze particle trajectories and statistical behaviors under various conditions, focusing on both the motions of individual particles and the collective evolution of bedforms, and our primary results include: 1. The incipient motion of particles is a gradual process that can occur before reaching the generally accepted critical Shields number. 2. The emergence and development of bedforms under varying conditions. 3. Observations on the relationship between particle movement characteristics and the shear conditions. These findings enhance our understanding of particle-scale dynamics in bedload transport, providing a foundation for evaluating and improving existing models for predicting transport rates.

How to cite: Li, X., Zhao, T., and Xu, B.:  Flow Characteristics and Particle Kinematics in Bedload Transport: a CFD-DEM investigation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15234, https://doi.org/10.5194/egusphere-egu25-15234, 2025.

Assessing particle-scale interactions and transport phenomena is essential yet complex within geophysical flows found in both natural and artificial settings. This research introduces the design, validation, and calibration of a spherical inertial sensor particle meticulously engineered to achieve full kinematic equivalence with a solid sphere. By employing Micro-Electro-Mechanical Systems Inertial Measurement Unit (MEMS-IMU) technology, this low cost 40 mm particle can measure triaxial acceleration up to ±16g and triaxial angular velocity up to ±2000°/s, operating at a high sampling rate of 1000 Hz over a duration of one hour. The sensor particle possesses a dual-layered spherical configuration deliberately crafted to ensure alignment in shape, density, center of mass, moment of inertia, and elastic modulus with that of a solid sphere. Its performance is rigorously assessed, validated, and calibrated through a series of physical experiments. Furthermore, a data enhancement technique grounded in lubrication theory is invented to mitigate technical challenges associated with accelerometer saturation and temporal resolution. This method enables our sensor particle to accurately capture particle collision processes within liquid environment, which proves challenging with conventional approaches. This investigation offers a foundational instrument for large-scale particle motion studies, such as those related to debris flows, facilitating, for the first time, the precise measurement of the dynamic behavior of individual particles within a substantial ensemble.

How to cite: An, Y., Jiao, J., and Zhang, L.: Spherical Inertial Sensor for Measuring Particle-Scale Interactions in Geomorphic Flows with Full Kinematic Equivalence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15433, https://doi.org/10.5194/egusphere-egu25-15433, 2025.

We have investigated the modeling of collisional bed-load transport with a focus on continuum approaches for granular flow. A frictional-collisional framework, combining the Coulomb model and the kinetic theory of granular flows, is proposed to address the limitations of classical kinetic theory, which fails to accurately reproduce results from coupled fluid–discrete simulations. These discrepancies are attributed to assumptions of negligible interparticle friction and the absence of a saltation model in continuum formulations. 

To guide model development, the fluctuating energy balance obtained from discrete simulations is systematically compared with kinetic theory predictions. The analysis reveals that interparticle friction significantly affects the radial distribution function and increases energy dissipation, aligning with previous findings. Additionally, a saltation regime is identified, causing deviations from the viscosity and pseudo-thermal diffusivity laws of kinetic theory in dilute regimes. 

Building on these insights, the two-fluid model is modified to incorporate interparticle friction and coupled with a saltation model. The results demonstrate that for inelastic, frictional particles, interparticle friction primarily governs energy dissipation, and the macroscopic granular flow behavior is independent of microscopic particle properties. The enhanced model successfully reproduces the 𝜇(𝐼) rheology in the dense regime of granular flow. Experimental validation confirms significant improvements in predicting granular flow behavior, highlighting the model’s effectiveness in capturing key physical processes. 

How to cite: Chauchat, J., Chassagne, R., and Bonamy, C.: A Continuum Framework for Modeling Frictional-Collisional Interactions in Bed-Load Transport: Insights from Discrete Element Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16152, https://doi.org/10.5194/egusphere-egu25-16152, 2025.

EGU25-17293 | ECS | Orals | GM2.7

Dispersion - Erosion Coupling in Landslides 

Jeevan Kafle, Bekha R. Dangol, and Shiva P. Pudasaini

Non-hydrostatic dispersive models can better describe the landslide motion. Following a dispersive wave equation and a mechanical erosion model for mass flows, here, we develop a novel dynamically coupled dispersion-erosion wave model that combines these two very essential complex processes. The newly developed model for landslide recovers the classical dispersive water waves and dispersive wave equation for landslide as special cases. We present several exact analytical solutions for the coupled dispersion-erosion model. These solutions are constructed for the time and spatial evolution of the flow depth. Solutions reveal that the dispersion and erosion are strongly coupled as they synchronously control the landslide dynamics. The results show that the wave dispersive wave amplifies with the increasing particle concentration, decreasing earth pressure, higher gravitational acceleration, increased slope angle and increased basal friction. The important novel understanding is that the intensity of the dispersive wave increases when erosion and dispersion are coupled. The results indicate the essence of proper selection of the initial and boundary conditions while solving applied and engineering problems associated with the dispersive - erosive mass transport. This provides the foundation for our understanding of the complex dispersion and erosion processes and their interplay.

How to cite: Kafle, J., Dangol, B. R., and Pudasaini, S. P.: Dispersion - Erosion Coupling in Landslides, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17293, https://doi.org/10.5194/egusphere-egu25-17293, 2025.

EGU25-18148 | Posters on site | GM2.7

The Fractal and Topological Metrics for Assessing Three-Dimensionality in Dune Morphology  

Sree Sai Prasad Bodapati and Venu Chandra

Dunes are ubiquitous in river, marine, desert and Martian environments. The flow of fluid 
over mobile bed results in evolution of dunes of different sizes and shapes. The shape of dune 
has critical role in sediment transport and interacting with flow. Earlier studies assumed the 
dune shape as a triangle (2-Dimensional) to study the flow field over dunes. However, dunes 
are highly three dimensional and their 3D patterns can increase the form drag compared with 
equivalent 2D dunes in similar flows. Pearson correlation, 2D spatial correlations are used to 
describe three dimensionality of dune in previous studies. A robust methodology to quantify 
3D bed forms and linking it to the flow needs to be developed. In this study, experiments are 
conducted to form 3D dunes on plane bed with non-uniform fine sand (d50 = 0.395 mm, σg = 
1.56) under sub critical flow conditions. The bed morphology is continuously monitored 
using ultrasonic ranging probes (URS) placed 5 cm c/c distance in 1 m wide flume. 
Experiments are performed till equilibrium state is achieved and continued further (2 hrs) to 
observe the bed changes. The equilibrium bed is measured at 2 cm resolution with a laser 
distance meter. The 3D velocity components and suspended sediment concentration are 
continuously measured using down looking Accoustic Doppler Velocimeter (25 Hz). Signal 
processing techniques are used to remove outliers, to smoothen the local fluctuations and 
identification of dune crest and troughs. In addition to 2D correlation and Pearson correlation 
coefficient, Fractal dimensions and topological metrics are also used to asses three 
dimensionality of the sediment bed. Roughness of the sediment bed is quantified using 
standard deviation of bed elevation. From the experiments, it was observed that three 
dimensionality is reduced with an increase in discharge. The spatial data is transformed into 
frequency domain. Periodicity of the process is analyzed from harmonics and spatially 
averaged spectrums. The height and length of dunes is modelled using exponential fits and 
observed a nonlinear growth of dunes. The flow measurements showed that the flow velocity 
in lobe region and turbulent kinetic energy in saddle region are increased. The mean sediment 
flux in the flow direction is directly proportional to the depth. Whereas, the turbulent fluxes 
exhibit an increasing trend up to 0.36–0.38 times the flow depth and then decrease with 
further increases in flow depth.

How to cite: Bodapati, S. S. P. and Chandra, V.: The Fractal and Topological Metrics for Assessing Three-Dimensionality in Dune Morphology , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18148, https://doi.org/10.5194/egusphere-egu25-18148, 2025.

EGU25-19135 | ECS | Orals | GM2.7

Quantifying Tidal Dune Morphodynamics at the Laboratory Scale: A Combined Measuring and Modelling Approach 

Gaetano Porcile, Dominique Mouazé, Pierre Weill, Aurélien Gangloff, and Anne-Claire Bennis

Understanding the morphodynamics of tidal dunes is essential for improving predictions of sediment transport and seabed evolution in coastal and estuarine environments. This study advances our understanding through a combined experimental and numerical investigation into the short-term morphodynamic evolution of laboratory-scale tidal dunes under controlled conditions.

Building on earlier flume experiments examining hydrodynamic interactions of reversing currents with fixed-bottom, sand-coated asymmetric compound dunes, we incorporated a cm-thick layer of unimodal sediment over the rigid dune models to simulate mobile-bed conditions. High-resolution Particle Image Velocimetry (PIV) was employed to capture detailed spatial and temporal dynamics of turbulent flows and the concurrent evolution of dune surfaces.

Complementary numerical modelling utilised the oceanographic circulation model CROCO, incorporating its non-hydrostatic solver and the USGS sediment transport module. The lab-scale model application was calibrated and validated against the laboratory measurements, demonstrating exceptional agreement in the short-term evolution of dune morphology. Key findings include the accurate replication of observed boundary layer dynamics, sediment transport mechanisms, and morphodynamic changes under reversing tidal currents. These experiments establish a solid benchmark for validating non-hydrostatic models of tidal dune morphodynamics.

This work underscores the transformative potential of integrating detailed physical experiments with advanced numerical models to refine our predictive capabilities for morphodynamic processes in tidal environments. The insights gained are particularly significant for coastal engineering and seabed mobility studies, with direct applications to the design and optimisation of offshore wind farm infrastructures.

How to cite: Porcile, G., Mouazé, D., Weill, P., Gangloff, A., and Bennis, A.-C.: Quantifying Tidal Dune Morphodynamics at the Laboratory Scale: A Combined Measuring and Modelling Approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19135, https://doi.org/10.5194/egusphere-egu25-19135, 2025.

EGU25-20382 | ECS | Orals | GM2.7

Submerged granular collapse: different cohesion strength and initial packing densities 

Rui Zhu, Zhiguo He, and Eckart Meiburg

We investigate the submerged cohesive collapse of cohesive granular columns, as a function of packing densities and cohesive force strength, via grain-resolving direct numerical simulations. We not only obtain the randomly packed granular columns but also the regular densely packed columns by Hexagonal close-packed (HCP) structure. The cohesive forces act to reduce the final runout distance of the collapsing column, which will no longer collapse when the cohesive force is larger than a critical value. This critical value decreases with the increase of the packing density. The cohesive forces significantly accelerate the contraction for loosely packed columns and decelerate the dilation for densely packed columns, resulting in a larger positive excess pore pressure and a smaller negative excess pore pressure, respectively. The collapsing column has distinct straight-like failure surfaces at the initial time, whose angle with the horizontal plane increases with the packing density. The force-chain network analysis indicates that the strong cohesive force chains form more easily in the failure region and have a larger size with increasing the cohesive force and packing density, which induces a larger macroscopic cohesive resistance. The cohesive force has a canceling effect on the normal contact force, which results in a smaller size for the contact force chains.

How to cite: Zhu, R., He, Z., and Meiburg, E.: Submerged granular collapse: different cohesion strength and initial packing densities, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20382, https://doi.org/10.5194/egusphere-egu25-20382, 2025.

EGU25-3501 | Orals | ST2.8

The pioneer Cluster mission 

Arnaud Masson, Philippe Escoubet, Detlef Sieg, Silvia Sanvido, Beatriz Abascal Placios, Stijn Lemmens, Bruno Sousa, and Helen Middleton

The Cluster mission will always be the first ever 4 spacecraft mission mapping the Earth magnetosphere in three dimensions. Launched in 2000 and originally planned to operate for two years, it has been orbiting Earth for more than two solar cycles. Over the course of its lifetime, its data have enabled the scientific community to conduct pioneer science in various aspects, including: plasma energization, energy transport and solar wind-magnetosphere-ionosphere interactions. Recent scientific highlights will be presented first, followed by the latest scientific objectives that have guided the Cluster mission operations from 2021 to 2024. Early September 2024, one spacecraft of this veteran constellation successfully re-entered in a controlled manner the Earth’s atmosphere. Some aspects of this re-entry will be presented.

How to cite: Masson, A., Escoubet, P., Sieg, D., Sanvido, S., Abascal Placios, B., Lemmens, S., Sousa, B., and Middleton, H.: The pioneer Cluster mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3501, https://doi.org/10.5194/egusphere-egu25-3501, 2025.

EGU25-3806 | ECS | Orals | ST2.8

Space Weather Investigation Frontier (SWIFT): Distinguishing between Local and Global Processes Driving Space Weather 

Mojtaba Akhavan-Tafti, Adam Szabo, Les Johnson, James Slavin, Tuija Pulkkinen, Dominique Fontaine, Susan Lepri, Emilia Kilpua, Ward Manchester, Rohan Sood, Omar Leon, Matti Ala-Lahti, Nishtha Sachdeva, Shirsh Soni, Lynn Wilson, and Lan Jian

Mesoscale heliospheric structures affecting the solar wind-magnetosphere coupling can be either injected by the Sun into the solar wind or generated locally in the near-Earth environment. These structures, ranging between tens to hundreds of Earth radii in scale, are observed in remote sensing observations of the solar corona, and in in-situ observations at Earth. However, resolving the formation, three-dimensional structure, and temporal evolution of these structures requires in-situ, multi-point observations, which existing (or planned) observatories do not provide. Here, we propose a groundbreaking mission concept, titled “Space Weather Investigation Frontier” (SWIFT), which utilizes flight-ready solar sail propulsion to enable continuous, in-situ observations along the Sun-Earth line at and inside the Lagrange point L1 (sub-L1). One sailcraft hub at sub-L1 and three identical nodes at L1 will fly in an optimized tetrahedron constellation to distinguish between local and global processes that drive space weather. To achieve this, SWIFT will investigate the spatial characteristics, temporal evolution, and geo-effectiveness of meso-scale solar wind structures as well as the substructures of macro-scale structures, such as interplanetary coronal mass ejections (ICMEs) and stream interaction regions (SIRs). In addition, SWIFT will provide real-time measurements of Earth-bound heliospheric structures, thus improving our current space weather forecasting lead-times by up to 40% –aligned with both NASA and NOAA's space weather priorities. The presentation will further highlight the SWIFT team’s 1) demonstration of the near-Earth formation and evolution of meso-scale solar wind structures using state-of-the-art global simulations, as well as 2) sailcraft charging analyses confirming the cleanliness of the sail for reliable, in-situ fields and plasma measurements.

How to cite: Akhavan-Tafti, M., Szabo, A., Johnson, L., Slavin, J., Pulkkinen, T., Fontaine, D., Lepri, S., Kilpua, E., Manchester, W., Sood, R., Leon, O., Ala-Lahti, M., Sachdeva, N., Soni, S., Wilson, L., and Jian, L.: Space Weather Investigation Frontier (SWIFT): Distinguishing between Local and Global Processes Driving Space Weather, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3806, https://doi.org/10.5194/egusphere-egu25-3806, 2025.

EGU25-5649 | Orals | ST2.8

Multi-scale processes of dayside magnetopause reconnection: a coordinated observation 

Enze Zhao, Malcolm Dunlop, Xiangcheng Dong, Xin Tan, Chunming Zhang, Huishan Fu, and C. Philippe Escoubet

We report an observation on 21 December 2019 when the Magnetospheric Multiscale (MMS) spacecraft encountered secondary magnetic reconnection located between two primary X-lines, at the low latitude magnetopause. Solar wind conditions provided by the Advanced Composition Explorer (ACE) spacecraft show that several, short IMF-Bz reversals occurred in this period. This caused a number of foreshock transients and magnetosheath perturbations, which were simultaneously observed by the Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft D and A. Under such influence, several small-scale flux transfer events (FTEs) with different sizes and axis orientations were observed by MMS, adjacent to an apparent X-line crossing. Meanwhile two larger-scale FTE signatures were also later observed afterwards by both Cluster 1 and 3 (located at high northern latitudes magnetopause), both with similar time delays of ~4 min from MMS FTEs. Notably, electron jets with different VL and VN were observed by MMS 1-3 adjacent to the flux ropes. We used multi-spacecraft Grad-Shafranov (GS) reconstruction to study the spatial structures of the flux ropes, also the relations to the electron jets. Our results improve our understanding of how solar wind influence the multi-scale processes of magnetopause reconnection, through foreshock transients and magnetosheath disturbance.

How to cite: Zhao, E., Dunlop, M., Dong, X., Tan, X., Zhang, C., Fu, H., and Escoubet, C. P.: Multi-scale processes of dayside magnetopause reconnection: a coordinated observation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5649, https://doi.org/10.5194/egusphere-egu25-5649, 2025.

EGU25-5814 | ECS | Posters on site | ST2.8

Shock Reformation Induced by Ion-scale Whistler Waves in Quasi-perpendicular Bow Shock 

Sibo Xu, Jiaji Sun, Shan Wang, Jinghuan Li, Xuzhi Zhou, Yufei Hao, Qiugang Zong, and Chao Yue

Studies have long suggested that shocks can undergo cyclical self-reformation as a result of shock nonstationarity. Until now, providing solid evidence for shock reformation in spacecraft observation and identifying its generating mechanisms remain challenging. In this work, by analyzing Magnetospheric Multiscale (MMS) spacecraft observations, we unambiguously identified shock reformation occurring in a quasi-perpendicular shock. A 2-D particle-in-cell simulation reproduces and explains the observed shock reformation. It reveals two distinct stages: in the early stage, whistler waves generated by the modified two-stream instability (MTSI) dominate the foot region, while whistler precursors driven by the gradient catastrophe instability dominate the ramp. In the later stage, MTSI-driven whistlers extend to the ramp and take over the role of reducing gradients, so precursors no longer develop. Both types of whistlers can result in shock reformation: one single wave period induces the magnetic field pile-up, ion accumulation and reflection, and upstream-pointing electric field, finally evolving into a new shock front. Our results give evidence that the shock reformation in the present regime can be driven by ion-scale whistler waves and demonstrate the detailed kinetic processes how it happens, providing valuable insights into the shock dynamics.

How to cite: Xu, S., Sun, J., Wang, S., Li, J., Zhou, X., Hao, Y., Zong, Q., and Yue, C.: Shock Reformation Induced by Ion-scale Whistler Waves in Quasi-perpendicular Bow Shock, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5814, https://doi.org/10.5194/egusphere-egu25-5814, 2025.

Understanding turbulence in space and astrophysical plasmas is critical for advancing our comprehension of complex systems governed by nonlinear dynamics. This study extends the application of the Markovian framework in small-scale turbulence in the Earth’s magnetosphere, with a particular focus on the solar wind – magnetosphere interaction observed by NASA Magnetospheric Multiscale (MMS) mission. We benefit from the exceptional resolution of the Fluxgate Magnetometer instrument as well as the Fast Plasma Investigation instrument onboard the MMS. The high temporal resolution, coupled with recent machine learning methods, allows one to identify the turbulent regions and magnetic reconnection events with great accuracy. Hence, the data are analyzed across diverse magnetospheric regions, enabling insights into turbulence-driven energy transfers. With the obtained measurements we could analyze the magnetic field gradients, turbulence intensity, and the plasma parameters. 

By employing the multi-scale probabilistic approach, we explore the turbulent cascade using conditional Probability Density Functions (cPDFs) and the Markovian properties of fluctuations, revealing new insights into the dynamics of energy transfer at sub-ion scales. Our results confirm the Markovian necessary and sufficient properties of the turbulent cascade across kinetic scales, emphasizing the significance of the Einstein-Markov (EM) scale and the intermittent nature of energy transfer to smaller scales. The derived Fokker-Planck equation in scale governs the evolution of cPDFs through drift and diffusion coefficients, which have been directly calculated from the empirical data. This employed framework captures key features of turbulence, including its hierarchical structure, deviations from self-similarity, and the phenomenon of intermittency, evidenced by non-Gaussian statistics and broadened PDF tails. These findings provide a robust description of the cascade process, from large-scale energy input to dissipation at smaller scales.

By investigating turbulence in two electron diffusion regions, where magnetic reconnection may occur, the highlighted Markovian framework and Fokker-Planck methodology are interestingly still viable to describe the complexity of turbulence processes. This gives promising insight into understanding the stochastic nature of reconnection-driven turbulence.

Despite some limitations, including the simplifying assumptions inherent to the Markovian framework and second-order Fokker-Planck equations, our results demonstrate its effectiveness in capturing the essence of kinetic-scale turbulence. The connection between scale-dependent statistics and underlying physical processes, such as intermittency and energy cascades, highlights the framework’s utility for both theoretical and observational studies. 

This work bridges statistical physics and plasma turbulence for analyzing scale-dependent phenomena in magnetospheric plasmas. We hope that by elucidating the interplay of order and randomness in these systems, our findings support the idea of extending stochastic modeling to higher-dimensional problems.

Acknowledgments: This work has been supported by the National Science Centre, Poland (NCN), through grant No. 2021/41/B/ST10/00823.

[1] W. M. Macek, D. Wójcik, & J. L. Burch, 2023, Magnetospheric Multiscale Observations of Markov Turbulence on Kinetic Scales, Astrophys. J. 943:152, https://doi.org/10.3847/1538-4357/aca0a0.
[2] W. M. Macek & D. Wójcik, 2023, Statistical analysis of stochastic magnetic fluctuations in space plasma based on the MMS mission, MNRAS, 526, 5779–5790, https://doi.org/10.1093/mnras/stad2584.
[3] D. Wójcik & W. M. Macek 2024, Testing for Markovian character of transfer of fluctuations in solar wind turbulence on kinetic scales, Phys. Rev. E 110, 025203, https://doi.org/10.1103/PhysRevE.110.025203.

How to cite: Wójcik, D. and Macek, W. M.: Testing For Universality of Markov Solar Wind Turbulence at the Earth’s Magnetosphere on Kinetic Scales Based on the MMS Mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6599, https://doi.org/10.5194/egusphere-egu25-6599, 2025.

EGU25-6739 | Orals | ST2.8

Wave-particle interactions in the outer regions of the dayside magnetosphere 

Ondrej Santolik, Benjamin Grison, and Jan Souček

Different types of electromagnetic waves propagate and interact with charged particles in the outer regions of the dayside magnetosphere. We review previous measurements of Polar, Cluster, Themis, MMS and Van Allen Probes spacecraft missions to show examples of these interactions. Whistler mode chorus and exohiss emissions occur up to the magnetopause on the dayside with increasing Poynting flux. Chorus is generated by a nonlinear mechanism based on the cyclotron resonance with low energy electrons, and accelerates relativistic electrons in the outer radiation belt. Its fine structure of subpackets discovered by the Cluster mission strongly influences these processes. Equatorial noise emissions are generated from the ion Bernstein modes, have distinct polarization properties of their magnetic field components,  and propagate below the lower hybrid frequency. These waves, sometimes also denoted as the magnetosonic waves, can accelerate energetic electrons and occur up to the outer boundaries of the magnetosphere on the dayside. Relatively rarely occurring Electromagnetic ion cyclotron (EMIC) waves are generated by a nonlinear mechanism from instable ion distributions and also interact with energetic electrons. Measurements show that their occurrence rates increase in the outer regions close to the dayside magnetopause. 

How to cite: Santolik, O., Grison, B., and Souček, J.: Wave-particle interactions in the outer regions of the dayside magnetosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6739, https://doi.org/10.5194/egusphere-egu25-6739, 2025.

EGU25-6783 | Posters on site | ST2.8

The Energetic Particle Experiment on the Plasma Observatory Daughter Spacecraft 

Malcolm W Dunlop, Vassilis Angelopoulos, Rami Vainio, Robert F Wimmer-Schweingruber, Demet Ulusen Aksoy, Ethan Tsai, Mark Prydderch, Jussi Lethi, William Grainger, Christopher Liu, Ryan Caron, Alex Steven, Oliver Bowett, Lars Berger, Svea Jürgensen, and Patrick Kühl

Plasma Observatory is a candidate mission of the European Space Agency (ESA) with a possible mission selection foreseen in 2026 and possible mission adoption in 2029. The mission aims to investigate cross-scale coupling and plasma energization across key regions of the magnetosphere, including: the bow shock, magnetopause, magnetotail and transition regions. To achieve this aim, Plasma Observatory will investigate the rich range of interesting plasma phenomena in these regions in the Earth’s magnetosphere, using a constellation of a mother and six daughter spacecraft. This allows configuration of the spacecraft in two nested tetrahedra to probe coupling on both ion and fluid scales. Since energetic particles are sensitive tracers of energization processes, altering the energy (or velocity) of both ions and electrons, measuring these effects in situ and at high cadence is of high importance for the mission. Energetic electrons and ions will be measured by the Energetic Particle Experiments (EPE) on the main (-M) and six daughter (-D) spacecraft. Here we present the EPE-D instrument, which is a compact, dual-particle telescope, solid state detector design based on ELFIN’s EPD instruments. Using three telescopes, it achieves near 3-D distributions for ions and electrons (135 x 360 deg). The development consists of deflecting magnets on the ion side (to screen out electrons) and a Lexan foil cover on electron side (to screen out low energy ions). The energy range (30-600 keV) for both species is targeted on low-end, suprathermal energies (minimising the effective gyro-scales for the computation of moments, PAD (e) and FDF determination), and so allowing spatial differences to be resolved. Detector layering is based on expected dynamic energy range and allows anti-coincident logic to be applied to separate out the higher energy species.

How to cite: Dunlop, M. W., Angelopoulos, V., Vainio, R., Wimmer-Schweingruber, R. F., Ulusen Aksoy, D., Tsai, E., Prydderch, M., Lethi, J., Grainger, W., Liu, C., Caron, R., Steven, A., Bowett, O., Berger, L., Jürgensen, S., and Kühl, P.: The Energetic Particle Experiment on the Plasma Observatory Daughter Spacecraft, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6783, https://doi.org/10.5194/egusphere-egu25-6783, 2025.

EGU25-8853 | ECS | Orals | ST2.8

Unique Multi-spacecraft constellation during active Kelvin-Helmholtz Instability 

Adriana Settino and Rumi Nakamura and the November 27, 2021 boundary event study team

We present observations of enhanced Kelvin-Helmholtz (KH) wave activity detected on November 27, 2021 between 05:00 - 6:30 UT, during predominantly southward IMF orientation, at the low-latitude magnetopause boundary by THEMIS and CLUSTER, both located on the magnetospheric side and separated by about 10 RE in the xy plane in the GSM system. Such a constellation of spacecraft and their multi-point measurements provides a unique opportunity to study the propagation of KH waves along the flank magnetopause and shed light on their evolution from the dayside (THEMIS location) to the nightside flank sector (Cluster location). Furthermore, the spacecraft separation enable us to recover information on the extent of the waves and the penetration of magnetosheath plasma into the magnetospheric side. Interestingly, such fluctuations were observed by all three THEMIS A, D and E spacecraft, whereas only two of the CLUSTER spacecraft (C1, C2) clearly observed them. In addition, C1 and C2 observed quite periodic fluctuations in the magnetic field, while THEMIS observed less periodic fluctuations separated by intervals of observation of relatively quiet magnetosheath plasma. These observations suggest a growth and evolution, or interaction between KH waves/vortices as they propagate tailward. Finally, a conjunction with MMS located at the same xy location as Cluster, but in the southern hemisphere, provides a better understanding of the surrounding plasma, as well as the effect of KH waves possibly propagating to the high-latitude magnetosphere.

How to cite: Settino, A. and Nakamura, R. and the November 27, 2021 boundary event study team: Unique Multi-spacecraft constellation during active Kelvin-Helmholtz Instability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8853, https://doi.org/10.5194/egusphere-egu25-8853, 2025.

Planetary bow shocks provide an excellent laboratory for studying shock physics. Over the past six decades, they have been extensively investigated in situ by various satellite missions aiming to study particle behavior and fields at both macro and micro scales. Despite significant progress, in situ measurements are limited to the spacecraft’s trajectory, providing only a partial description of the shock’s 3D structure. To address this problem, we can combine these measurements with kinetic plasma simulations, which can significantly enhance our understanding of shock physics. Fully kinetic methods, such as Particle-in-Cell (PIC) simulations, have the capability to describe the evolution of shocks at ion scales while also resolving the dynamics of electrons. However, to cover the necessary spatial and temporal scales, PIC simulations often require the use of unrealistic numerical parameters, such as artificially high shock velocities and reduced ion-to-electron mass ratios. These approximations introduce additional challenges because various aspects of shock microphysics—such as parameters of driven instabilities, heating mechanisms, and particle acceleration—exhibit distinct dependencies on these numerical parameters. This discrepancy complicates direct comparisons between PIC simulations and in situ measurements. To mitigate these issues, rescaling procedures tailored to specific phenomena are necessary. Here, we address the problems of magnetic field amplification, electron heating, and electrostatic waves, each requiring its own distinct set of rescaling procedures.

How to cite: Bohdan, A.: Bridging observations and simulations: challenges in planetary bow shock studies, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10244, https://doi.org/10.5194/egusphere-egu25-10244, 2025.

EGU25-10260 | ECS | Posters on site | ST2.8

Investigating energy conversion at the electron scales in Earth's magnetotail 

Giulia Cozzani, Matthieu Kretzschmar, and Paul Cassak

Magnetic reconnection is a fundamental plasma process that converts electromagnetic energy into bulk kinetic and thermal energy of the plasma through topological rearrangement of the magnetic field. This process is often accompanied by kinetic instabilities and wave activity, which can influence energy conversion. The electron firehose instability (EFI) is one such kinetic instability, which arises when the electron population has significant temperature anisotropy, and the parallel component of the temperature sufficiently exceeds the perpendicular component relative to the background magnetic field. The plasma in the reconnection outflow region can be unstable to the EFI and the presence of EFI-generated waves could potentially modify the energy distribution in the plasma.

We use data from the NASA Magnetospheric Multiscale (MMS) mission in Earth's magnetotail to investigate energy conversion associated with magnetic reconnection in different regions, including the Electron Diffusion Region (EDR) and the reconnection outflow hosting EFI-generated waves. To quantify energy conversion, we analyze various measures such as J.E (where J is the current density and E is the electric field), pressure-strain interaction, and the Higher-ORrder Non-Equilibrium Terms (HORNET) power density.

How to cite: Cozzani, G., Kretzschmar, M., and Cassak, P.: Investigating energy conversion at the electron scales in Earth's magnetotail, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10260, https://doi.org/10.5194/egusphere-egu25-10260, 2025.

EGU25-10320 | ECS | Orals | ST2.8

Particle Energization Associated With Foreshock Transients: Results From a Hybrid-Vlasov Simulation and MMS Observations 

Souhail Dahani, Lucile Turc, Shi Tao, Veera Lipsanen, Jonas Suni, Yann Pfau-Kempf, Minna Palmroth, Daniel Gershman, Roy Torbert, and James Burch

The interaction of solar wind discontinuities with reflected solar wind particles upstream of Earth's bow shock leads to the formation of large scale transient phenomena such as Foreshock Bubbles (FBs) and hot flow anomalies. These transient phenomena play an important role in accelerating and energizing plasma and could have global impacts on the near-Earth environment. Direct derivations from the Vlasov-Maxwell equation provide the equations that describe the temporal evolution of the kinetic and thermal energy. In this ongoing study, we investigate the behavior of the fluid energy terms that directly affect the evolution of the kinetic and thermal energy associated with these transients, with a particular focus on FBs. Specifically, we analyze the behavior of these energy terms in different sub-regions of the FB, including its core, sheath, and the shock created by its expansion. We employ a 2D global hybrid-Vlasov simulation performed with the Vlasiator model and compare the numerical results with a statistical study of FBs observed by the Magnetospheric MultiScale (MMS) mission. We discuss the role of FBs in accelerating, heating the plasma and producing or annihilating magnetic energy. 

How to cite: Dahani, S., Turc, L., Tao, S., Lipsanen, V., Suni, J., Pfau-Kempf, Y., Palmroth, M., Gershman, D., Torbert, R., and Burch, J.: Particle Energization Associated With Foreshock Transients: Results From a Hybrid-Vlasov Simulation and MMS Observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10320, https://doi.org/10.5194/egusphere-egu25-10320, 2025.

EGU25-11029 | ECS | Orals | ST2.8

Identifying magnetotail jet fronts in a 6D global hybrid-Vlasov simulation 

Lauri Pänkäläinen, Giulia Cozzani, Markus Battarbee, Urs Ganse, Yann Pfau-Kempf, Jonas Suni, and Minna Palmroth

Magnetic reconnection in Earth's magnetotail is thought to create bursty bulk flows (BBFs), short-lived plasma bulk velocity enhancements in the magnetotail's central plasma sheet (CPS) region. Closely related to BBFs are dipolarization fronts (DFs), sudden increases in Bz, the magnetic field component aligned with Earth's magnetic dipole axis. Both phenomena affect energy distribution and flux transport in the magnetotail.

We demonstrate novel methods of identifying BBFs and DFs in a 3D global magnetospheric simulation and present results for multiple case studies. BBFs and DFs are searched for in a simulation conducted using Vlasiator, a global magnetospheric hybrid-Vlasov code where ions are modeled using distribution functions and electrons are treated as a charge-neutralizing fluid. DFs are identified using a magnetic field time derivative threshold dBz /dt > 0.35 nT/s. BBFs are defined based on a velocity threshold, and they are studied on a case-by-case basis. Tailward DFs (anti-dipolarization fronts) are found at magnetic islands, while earthward DFs are mostly seen in finger-like structures of high earthward bulk velocity alongside BBFs. Signatures registered as BBFs in spacecraft view also originate due to moving reconnection locations and movement of the current sheet within the CPS while the reconnection outflow stays roughly constant. The results show that rapid Bz variations in the simulation have multiple sources, and similar satellite measurements of BBFs can arise from different physical phenomena. The findings may help with interpreting satellite observations in the magnetotail.

How to cite: Pänkäläinen, L., Cozzani, G., Battarbee, M., Ganse, U., Pfau-Kempf, Y., Suni, J., and Palmroth, M.: Identifying magnetotail jet fronts in a 6D global hybrid-Vlasov simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11029, https://doi.org/10.5194/egusphere-egu25-11029, 2025.

EGU25-11098 | ECS | Orals | ST2.8

Instabilities of the magnetotail current layer in hybrid-Vlasov simulations of the Earth’s magnetosphere. 

Ivan Zaitsev, Giulia Cozzani, Markku Alho, Konstantinos Horaites, Hongyang Zhou, Sanni Hoilijoki, Yann Pfau-Kempf, Markus Battarbee, Urs Ganse, Konstantinos Papadakis, Jonas Suni, Venla Koikkalainen, Lucile Turc, and Minna Palmroth

 On the macroscale, the large-scale magnetic field structure governs the magnetotail current layer. At the same time, it must be supported by the self-consistent dynamics of charged particles. While the current layer reaches a critical state, microscale processes start to play a leading role by triggering kinetic instabilities. These instabilities drive changes in large-scale magnetic topology and particle energization.

 This study examines the instabilities of the Earth's magnetotail current layer using global hybrid-Vlasov simulations (Vlasiator). In our simulation, the southward interplanetary magnetic field causes dayside reconnection which leads to the accumulation of magnetic flux on the night side and the magnetotail current sheet thins down to ~5 proton inertial lengths. The current layer undergoes reconnection accompanied by the formation of multiple X-lines initiated by tearing instability. During the formation of the X-lines, we observe crescent-shaped proton velocity distributions as the signature of resonance interaction of the demagnetized population with the reconnection electric field. The tearing instability manifests as the filamentation of the electric current, appearing as a chain of plasmoids extending along the Sun-Earth direction. Fourier analysis of the perturbed electric current reveals a tearing growth time on the order of ~40 proton gyroperiods for plasmoids with a characteristic size of ~30 skin depths. 

 As the tearing instability evolves, the kinking of the current layer gets more prominent on the duskward side of the tail. The kink instability leads to the excitation of the flapping-type waves developing across the tail. The wavelength of the flapping oscillations is ~ 15 proton skin depths, and the growth time is ~80 proton gyroperiods. The active thermalization of the crescent-shaped proton distributions is associated with the development of kink instability.

How to cite: Zaitsev, I., Cozzani, G., Alho, M., Horaites, K., Zhou, H., Hoilijoki, S., Pfau-Kempf, Y., Battarbee, M., Ganse, U., Papadakis, K., Suni, J., Koikkalainen, V., Turc, L., and Palmroth, M.: Instabilities of the magnetotail current layer in hybrid-Vlasov simulations of the Earth’s magnetosphere., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11098, https://doi.org/10.5194/egusphere-egu25-11098, 2025.

EGU25-11134 | ECS | Orals | ST2.8

J-Filtering: A Novel Multipoint Technique for Current Distribution Analysis in Space Plasmas   

Mehul Chakraborty, Jean-Louis Pincon, and Matthieu Kretzschmar

Both the interplanetary medium and the near-Earth space are filled with plasmas and a key remaining question in space physics is the understanding of the processes governing the energization of both particles and waves in space plasmas. Measurements of the fields in space plasmas exhibit temporal and spatial variations across all observed scales. Single-satellite measurements provide only a partial picture because they cannot capture the details of these variations. Multipoint missions, particularly the four-satellite tetrahedron configurations of CLUSTER  and MMS , were launched to overcome this limitation. Specialized techniques for multipoint data analysis have been developed. Among them, the Curlometer exploits the magnetic field measurements of the individual spacecraft magnetometers and uses Maxwell-Ampere's law to estimate the current density (J) through the tetrahedron formed by the four-spacecraft constellation. However, it assumes a linear spatial variation of the magnetic field across the spacecrafts, which actually seriously limits its applicability in space plasmas. To overcome the limitations of the Curlometer, we are proposing a new technique called J-Filtering (where J represents current density) for measuring and visualizing local current distributions in space. The idea behind J-Filtering is to borrow the principle of optimal filter determination from the K-filtering method, which was developed for the CLUSTER mission. Here, the filters are defined to allow identification of the current structures that are responsible for the magnetic fields measured by the spacecrafts of the constellation . We will present the principles of J-Filtering and its first applications to spacecraft data from CLUSTER, showing in particular its validation by comparison with the Curlometer results when the linear spatial variation condition is assumed. We will also present results obtained by applying the techniques to MMS data specifically for thin current sheets at reconnection sites where the Curlometer method can be not valid.

How to cite: Chakraborty, M., Pincon, J.-L., and Kretzschmar, M.: J-Filtering: A Novel Multipoint Technique for Current Distribution Analysis in Space Plasmas  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11134, https://doi.org/10.5194/egusphere-egu25-11134, 2025.

Plasma energization and energy transport are ubiquitous in cosmic plasmas. The Earth’s Magnetospheric System is a key example of a highly structured and dynamic cosmic plasma environment where massive energy transport and plasma energization occur and can be directly studied through in situ spacecraft measurements. Despite the large amount of available in situ observations, however, we still do not fully understand how plasma energization and energy transport work. This is essential for assessing how our planet works, including space weather science, and is also important for the comprehension of distant astrophysical plasma environments. In situ observations, theory and simulations suggest that the key physical processes driving plasma energization and energy transport occur where plasma on fluid scales couple to the smaller ion kinetic scales, at which the largest amount of electromagnetic energy is converted into energized particles. Remote observations currently cannot access these scales, and existing multi-point in situ observations do not have a sufficient number of observation points. Plasma Observatory will be the first mission having the capability to resolve scale coupling in the Earth’s Magnetospheric System through measurements at seven points in space, covering simultaneously the ion and the fluid scales where the strongest plasma energization and energy transport occurs: the foreshock, bow shock, magnetosheath, magnetopause, magnetotail current sheet, and transition region. By resolving scale coupling in plasma processes such as shocks, magnetic reconnection, turbulence, plasma instabilities, plasma jets, field-aligned currents and their combination, these measurements will allow us to answer the two Plasma Observatory science questions (Q1) How are particles energized in space plasmas? and (Q2) Which processes dominate energy transport and drive coupling between the different regions of the Earth’s Magnetospheric System? Going beyond the limitations of Cluster, THEMIS and MMS multi-point missions, which can only resolve plasma processes at individual scales, Plasma Observatory will transform our understanding of the plasma environment of our planet with a major impact on the understanding of other planetary plasmas and astrophysical plasmas too. 

How to cite: Retinò, A. and the The Plasma Observatory Team: Unveiling Plasma Energization and Energy Transport in the Earth’s Magnetospheric System through Multi-Scale Observations: the Science of the ESA M7 Plasma Observatory Mission Candidate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11432, https://doi.org/10.5194/egusphere-egu25-11432, 2025.

EGU25-11741 | Posters on site | ST2.8 | Highlight

The Heliophysics Accords: A blueprint for a unified, worldwide, Heliophysics community 

Emil Kepko and the COSPAR Task Group on Establishing an International Geospace Systems Program

The recently released US Heliophysics Decadal Survey recommends that the identity of the solar and space physics community needs to be solidified, in order to unify under a common and recognized name. This would greatly benefit collaboration, recruitment, education, and public outreach. The obvious identify for our field is Heliophysics. Heliophysics is the study of the Sun and its effects throughout the solar system. It covers an incredible range of scales, from plasma physics at the electron scale to the boundary that separates our solar system from interstellar space. The components of Heliophysics sit at the boundaries of Earth science, Planetary science, and Astrophysics: Aeronomy at the boundary of our atmosphere and space; Solar physics at the boundary of the sun and interplanetary space; Heliospheric science at the boundaries of the solar wind and planets, and at the boundary of our solar system and interstellar space. Space plasma physics, the science of how ionized and partially ionized plasmas behave in the presence of electromagnetic fields, undergirds the field. Many of the biggest unanswered science questions that remain across Heliophysics center around the interconnectivity of the different physical systems, and the role of mesoscale dynamics in modulating, regulating, and controlling that interconnected behavior. Answering these long-standing questions on the Sun-Heliosphere and Geospace as system-of-systems requires a coordinated, deliberate, worldwide scientific effort, akin to the highly successful ISTP program. In this talk we describe the next steps in creating a unified, worldwide, vibrant Heliophysics community, building upon the previous efforts of ISTPNext. This next step will put in place concrete elements to usher in the next era of Heliophysics, focused on cross-scale and cross-regional coupling, combining in situ, remote and ground-based observations with state-of-the-art modeling, amongst the worldwide Heliophysics community.  

How to cite: Kepko, E. and the COSPAR Task Group on Establishing an International Geospace Systems Program: The Heliophysics Accords: A blueprint for a unified, worldwide, Heliophysics community, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11741, https://doi.org/10.5194/egusphere-egu25-11741, 2025.

EGU25-11909 | Posters on site | ST2.8

Science Study Team Working Groups of the ESA M7 Mission candidate Plasma Observatory  

Matthew Taylor, Federica Marcucci, and Alessandro Retino and the Plasma Observatory WG team

We know that plasma energization and energy transport occur in large volumes of space and across large boundaries in space. However, in situ observations, theory and simulations indicate that the key physical processes driving energization and energy transport occur where plasma on fluid scales couple to the smaller kinetic scales, at which the largest amount of electromagnetic energy is converted into energized particles. Energization and energy transport involve non-planar and non-stationary plasma structures at these scales that have to be resolved experimentally. Remote observations currently cannot access these scales, and existing multi-point in situ observations do not have a sufficient number of observations points. 

The Plasma Observatory (PO) multi-scale mission concept is a candidate for the ESA Directorate of Science M7 mission call, currently in a Phase A study. Plasma Observatory will be the first mission to have the capability to resolve scale coupling and non-planarity/non-stationarity in plasma energization and energy transport.

During the Phase A study, Scientific guidance of the mission is provided by the ESA nominated Science Study Team (SST). In support of this group is the Cross Disciplinary working group, who provide close support to the SST and study activities. To ensure a broad input and wide community involvement the SST has organised several working groups in order to expand the community and citizen science involvement. These working groups cover Ground-based coordination, Public outreach and Numerical Simulation, multipoint and advanced data analysis methods, plasma astrophysics and scientific synergies.

This paper provides an overview of these WG and how you can get involved in Plasma Observatory.

How to cite: Taylor, M., Marcucci, F., and Retino, A. and the Plasma Observatory WG team: Science Study Team Working Groups of the ESA M7 Mission candidate Plasma Observatory , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11909, https://doi.org/10.5194/egusphere-egu25-11909, 2025.

EGU25-11978 | ECS | Posters on site | ST2.8

Progress and Updates from the Plasma Observatory Synergies/Additional Science Working Group 

Simone Benella, Jean Francois Ripoll, Cecilia Norgren, Oliver Allanson, Lorenzo Biasiotti, Sara Gasparini, Matina Gkioulidou, Hantao Ji, Yoshi Miyoshi, Rumi Nakamura, Alexander Pitna, Dorota Przepiórka-Skup, Adriana Settino, Marina Stepanova, Sergio Toledo-Redondo, Drew Turner, and Emiliya Yordanova

Plasma Observatory (PO) is one of the three Class-M7 ESA missions currently in Phase A, and is designed to investigate fundamental processes at the base of energization and energy transport, such as collisionless shocks, plasma jets, wave, turbulence, and magnetic reconnection by gathering unprecedented multipoint and multiscale measurements of near-Earth plasma environments. The mission concept consists of a constellation of seven spacecraft in a double nested tetrahedron formation with a common vertex. The key science regions (KSRs) of the PO mission are Earth bow shock, foreshock, magnetosheath, magnetopause, tail plasma sheet and transition region. However, additional science regions (ASRs) such as inner magnetosphere, flank magnetopause, and pristine solar wind will be traversed by the constellation during the orbit, thus allowing for additional scientific targets. In this context, the Synergies/Additional Science Working Group aims to systematically investigate the major scientific advancements that can be achieved by leveraging the PO constellation in the various regions explored outside the KSRs, and to maximize the scientific return of the mission by broadening the PO science community by including space plasma scientists from other fields.

Since the magnetospheric system is a highly dynamic environment subjected to the solar wind forcing, especially during solar wind transient events, important physical processes can be studied by observing the magnetospheric response to them. New multiscale measurements of fields and particles at more than four points, for instance, are crucial for investigating the magnetosphere-ionosphere coupling for different levels of geomagnetic activity. Moreover, PO will provide measurements at the edge of the outer radiation belt, allowing to study fundamental plasma processes such as particle acceleration, transport and loss, wave-particle interactions and so forth. Large scale phenomena developing in ASRs such as solar wind and flank magnetopause, such as turbulence, reconnection, and instabilities are connected to ion and sub-ion scales where the energy is dissipated. In this spirit, simultaneous multiscale observations gathered in the ASRs are crucial for investigating the connection between MHD-scale plasma structure dynamics, turbulent energy transfer and the energy conversion occurring at small-scales. Beyond the ASRs observed in situ by the spacecraft constellation, there are strong synergies with laboratory activities. How does magnetic reconnection couple global MHD scales to local dissipation scales is an outstanding open question, some aspects of which can be addressed with the support of current and upcoming multiscale laboratory experiments that are, therefore, highly relevant for PO scientific objectives.

This contribution summarizes all the recent advancements made regarding the Synergies/Additional Science Working Group activities for PO and will discuss inputs and future perspectives supporting the mission Phase A.

How to cite: Benella, S., Ripoll, J. F., Norgren, C., Allanson, O., Biasiotti, L., Gasparini, S., Gkioulidou, M., Ji, H., Miyoshi, Y., Nakamura, R., Pitna, A., Przepiórka-Skup, D., Settino, A., Stepanova, M., Toledo-Redondo, S., Turner, D., and Yordanova, E.: Progress and Updates from the Plasma Observatory Synergies/Additional Science Working Group, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11978, https://doi.org/10.5194/egusphere-egu25-11978, 2025.

EGU25-12554 | ECS | Orals | ST2.8

Empirical Measurement of Diffusive Heating across Earth’s Bow Shock 

Tamar Ervin, Trevor Bowen, Alexandros Chasapis, Alfred Mallet, Philip Isenberg, Kristopher Klein, and Stuart Bale

We use high cadence observations of velocity distribution functions (VDFs) from the Magnetospheric Multiscale Mission (MMS) to empirically estimate diffusion coefficients and heating rates in a crossing of the Earth’s bow shock. We approximate the observed VDFs using non-parametric representations and evaluate the gradients of the modeled VDFs (GPR-VDF) to empirically estimate diffusion coefficients. This allows us to have a better representation of the non-thermal features of the distribution functions. We invert the proton guiding center equation to get estimates of diffusion coefficients and proton heating rates. We compare these results with theoretical models and simulations of stochastic heating, heating via cyclotron or Landau damping, and other heating methods to constrain the heating mechanism(s) at work across the shock. Our approach allows for an estimate from observations of collisionless heating rates within a kinetic framework and discussion of the mechanism(s) at work. This methodology could be applied to future multipoint measurements in the magnetosphere (e.g. Plasma Observatory) to study heating across shocks and other regions of interest. 

How to cite: Ervin, T., Bowen, T., Chasapis, A., Mallet, A., Isenberg, P., Klein, K., and Bale, S.: Empirical Measurement of Diffusive Heating across Earth’s Bow Shock, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12554, https://doi.org/10.5194/egusphere-egu25-12554, 2025.

EGU25-12644 | ECS | Posters on site | ST2.8

The Energetic Particle Experiment on the Plasma Observatory Mother Spacecraft 

Svea Jürgensen, Robert F Wimmer-Schweingruber, Lars Berger, Patrick Kühl, Malcolm Wray Dunlop, Rami O Vainio, and Vassilis Angelopoulos

Plasma Observatory is a candidate mission of the European Space Agency (ESA) with a possible selection foreseen in 2026 and a launch in 2037. It aims to investigate the plasma coupling across different scales. To achieve this aim, Plasma Observatory will investigate different regions in the Earth’s magnetosphere which is rich in many interesting plasma phenomena. It consists of a mother and six daughter spacecraft. This allows to configure the spacecraft in two nested tetrahedra to investigate cross-scale coupling.

Energetic particles are sensitive tracers of processes which can alter the energy (or velocity) of ions and electrons. It is thus of high importance to measure them in situ at high cadence. They are bound to magnetic field lines but can be scattered onto others by various processes.

Energetic electrons and ions will be measured by the Energetic Particle Experiments (EPE) on the main (M) and six daughter (D) spacecraft. Here we present different instrument concepts for EPE-M, all of which which cover the energy range from 30 keV – 600 keV for electrons and up to 8 MeV for ions. The current (baseline) design utilizes the foil-magnet technique to separate electrons from ions. The experiment consists of two sensors each with two bidirectional telescopes and thus has eight viewing directions. Together with the spacecraft spin (2 rpm) EPE-M covers a field of view of nearly 4π steradians. Higher time resolution is possible at reduced angular resolution. Alternative design concepts have been derived and are presented as well.

How to cite: Jürgensen, S., Wimmer-Schweingruber, R. F., Berger, L., Kühl, P., Dunlop, M. W., Vainio, R. O., and Angelopoulos, V.: The Energetic Particle Experiment on the Plasma Observatory Mother Spacecraft, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12644, https://doi.org/10.5194/egusphere-egu25-12644, 2025.

EGU25-13482 | Posters on site | ST2.8

The Ion Mass Spectrometer instrument for Plasma Observatroy – IMS 

Harald Kucharek, Maria Federica Marcucci, Alessandro Retino, Benoit Lavraud, Lynn Kistler, Johan DeKeyser, Andre Galli, James Bundock, and Jean-Denis Techer

The overarching goal of the Plasma Observatory Missions is to use multiscale multi-spacecraft observations to investigate in detail plasma energization and plasma transport in the near-Earth region. Thus, the prime goals of that mission are: How are particles energized in that plasma environment? And what processes are dominant in transporting Energy in the Magnetospheric System.

The achieve these science goals electromagnetic fields and three-dimensional particle distributions will be measured in high resolution and accuracy. IMS (the Ion Mass Spectrometer) will measure the full three-dimensional distribution functions of near-Earth main ion species (H+, He+, He++ and O+) at high time resolution (~150 ms for H+ , ~ 300 ms for He++) with energy resolution down to ~10% in the range 10 eV/q to 30 keV/q and angular resolution _ ~10 .

Such high time resolution is achieved by mounting multiple sensors around the spacecraft body, in similar fashion to the MMS/FPI instrument. Each sensor combines a top-hat electrostatic analyser with deflectors at the entrance together with a time-of-flight section to perform mass selection. IMS electronics includes a fast sweeping high voltage board that is required to make measurements at high cadence. Ion detection includes Micro Channel Plates (MCP) combined with Application-Specific Integrated Circuits (ASICs) for charge amplification, discrimination and time-to-digital conversion (TDC). IMS will be designed to address directly many of the Plasma Observatory science objectives, in particular ion heating and acceleration by turbulent fluctuations in foreshock, shock and magnetosheath regions. In this presentation we will report on initial performance measurements of the IMS instrument and relate these mensurements to potential recordings at keys science areas.

How to cite: Kucharek, H., Marcucci, M. F., Retino, A., Lavraud, B., Kistler, L., DeKeyser, J., Galli, A., Bundock, J., and Techer, J.-D.: The Ion Mass Spectrometer instrument for Plasma Observatroy – IMS, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13482, https://doi.org/10.5194/egusphere-egu25-13482, 2025.

EGU25-14456 | Orals | ST2.8

Effects of Kelvin-Helmholtz-like waves on high-latitude magnetospheric boundary dynamics 

Rumi Nakamura and Adriana Settino and the November 27, 2021 event study team

On November  27 2021, between 05 and 10 UT, when THEMIS and Cluster were located near the dusk-side low-latitude magnetopause and observed several periods of enhanced  Kelvin-Helmholtz (KH) wave activity, MMS crossed the magnetopause in the southern hemisphere near the dusk-side terminator close to the local time of Cluster. IWF was predominantly southward at the beginning of the interval and was mainly northward after 07:00 UT. This interval coincides with the Earth-flyby of Solar Orbiter, which traversed the nightside magnetosphere and encountered the dusk side tail-flank boundary region. In this presentation, we focus on the MMS observations between 8:15-9:15 UT when MMS encountered flow-shear boundaries between tailward flowing lobe-like plasma and Earthward moving cold dense plasma sheet-like region mixed with hot ions inside the high-latitude magnetosphere. The latter region contains density/temperature fluctuations comparable to KH-like wave disturbance observed at the magnetopause by Cluster during the same interval.  Typically KH disturbances are observed between cold-dense magnetosheath-like plasma and magnetospheric plasma. However, during this interval MMS was located at the boundary between plasma sheet like-hotter plasma and colder lobe-like sparse plasma. We discuss the external and internal interaction processes that may explain these boundary disturbances.  The unique constellation of fleet of spacecraft fleets, covering different magnetospheric boundaries simultaneously enable us to study the effect of the KH-like magnetopause disturbances on the dynamics of the dusk-side magnetosphere in an extended region.

How to cite: Nakamura, R. and Settino, A. and the November 27, 2021 event study team: Effects of Kelvin-Helmholtz-like waves on high-latitude magnetospheric boundary dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14456, https://doi.org/10.5194/egusphere-egu25-14456, 2025.

EGU25-15349 | Posters on site | ST2.8

Ion behaviour in the vicinity of ballooning-interchange heads 

Evgeny V. Panov, Rumi Nakamura, and Wolfgang Baumjohann

Comparison of THEMIS spacecraft observations with kinetic simulations suggested that the kinetic Ballooning/Interchange Instability (BICI) may lead to erosion and thinning of the magnetotail current sheet at fluid scales due to side vorticity and associated an FLR effect and at ion scales by means of EMIC waves. The FLR effect may lead to ion temperature asymmetry on the two sides of BICI heads in the course of ion redistribution between the dusk- and dawnside vortices around the neutral sheet. On top of that, the EMIC waves may propagate in both azimuthal directions and modulate the ion density and velocity above and below the neutral sheet. As this activity may be important for turning Bz southward and possibly initiating magnetic reconnection in the magnetotail, we show high-resolution MMS ion observations with signatures of the two processes now in the MMS magnetotail bursty bulk flow observations and aim at finding evidence that the field and particle behaviour was caused by the two effects.

How to cite: Panov, E. V., Nakamura, R., and Baumjohann, W.: Ion behaviour in the vicinity of ballooning-interchange heads, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15349, https://doi.org/10.5194/egusphere-egu25-15349, 2025.

The formation of energetic electrons in relation to high speed flows in magnetotail has been observed by multiple missions. Here we focus on the formation of most energetic electron events. The physical mechanism how they are accelerated is still unclear. We report one of the most energetic electron events of the Cluster mission observations. The very high flux of  energetic electrons is observed at about 10 Re in magnetotail, associated with bursty bulk flows and rebound flows as observed by different Cluster spacecraft separated on the fluid scale. Understanding this event helps us better demonstrate how most energetic electrons are accelerated in the magnetotail. However, due to the limitation of large fluid-scale separation of the spacecraft, we can not address the physical mechanisms at the small ion scales, that is critical for understanding the energetic electron acceleration mechanisms.  We speculate how future multi-scale observations would allow us to make significant improvement in our understanding of the physics of energetic electron acceleration.

How to cite: Gai, C. and Vaivads, A.: Cluster Observations of the Most Energetic Electron Event Associated with Earthward and Tailward Flows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16439, https://doi.org/10.5194/egusphere-egu25-16439, 2025.

EGU25-16777 | Posters on site | ST2.8

The SCM instrument for the ESA Plasma Observatory mission 

Olivier Le Contel, Matthieu Kretzschmar, Alessandro Retino, Fatima Mehrez, Guillaume Jannet, Dominique Alison, Claire Revillet, Laurent Mirioni, Clémence Agrapart, Gérard Sou, Nicolas Geyskens, Christophe Berthod, Thomas Chust, Matthieu Berthomier, Cécile Fiachetti, Yuri Khotyaintsev, Vicki Cripps, and Maria federica Marcucci

The proposal of the Plasma Observatory mission was selected for a competitive phase A with two other missions in the framework of the seventh call for medium mission (M7) organized by ESA. The mission selection is planned in 2026 for a launch in 2037. Its main objectives are to unveil how are particles energized in space plasma and which processes dominate energy transport and drive coupling between the different regions of the terrestrial magnetospheric system? The mission consists of seven satellites, a main platform (mothercraft, MSC) and six smaller identical satellites (daughtercraft) evolving along an equatorial elliptical orbit with an apogee ~17 and a perigee ~8 Earth radii. The seven satellites will fly forming two tetraedra and allowing simultaneous measurements at both fluid and ion scales. The mission will include three key science regions: dayside (solar wind, bow shock, magnetosheath, magnetopause), nightside transition region (quasidipolar region, transient near-Earth current sheet, field-aligned currents, braking flow region) and the medium magnetotail (near-Earth reconnection region, fast flow formation region). Plasma Observatory mission is the next logical step after the four satellite magnetospheric missions Cluster and MMS. The search-coil magnetometer (SCM), strongly inherited of the SCM designed for the ESA JUICE mission, is only included in the Fields instrument suite of the MSC. SCM will be delivered by LPP and LPC2E and will provide the three components of the magnetic field fluctuations in the [0.1Hz-8kHz] frequency range, after digitization by the Low frequency Receiver (LFR) within the Field and Wave Processor (FWP), relevant for the three Key science regions. It will be mounted on a 6m boom and will allow to reach the following sensitivities [10-3, 1.5x10-6, 5x10-9, 10-10, 5x10-10] nT2/Hz at [1, 10, 100, 1000, 8000] Hz. Associated with the electric field instrument (EFI), SCM will allow to fully characterize the wave polarization and estimate the direction of propagation of the wave energy. These measurements are crucial to understand the role of electromagnetic waves in the energy conversion processes, the plasma and energy transport, the acceleration and the heating of the plasma.

 

How to cite: Le Contel, O., Kretzschmar, M., Retino, A., Mehrez, F., Jannet, G., Alison, D., Revillet, C., Mirioni, L., Agrapart, C., Sou, G., Geyskens, N., Berthod, C., Chust, T., Berthomier, M., Fiachetti, C., Khotyaintsev, Y., Cripps, V., and Marcucci, M. F.: The SCM instrument for the ESA Plasma Observatory mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16777, https://doi.org/10.5194/egusphere-egu25-16777, 2025.

EGU25-17806 | ECS | Posters on site | ST2.8

Investigating structures through gradient tensors in turbulent space plasmas: invariants’ evolution equations and Schur decomposition 

Virgilio Quattrociocchi, Giuseppe Consolini, Massimo Materassi, and Simone Benella

The availability of multi-point in situ data from space missions orbiting in solar wind and near-Earth environments offers valuable insights into fundamental physical phenomena such as shocks, magnetic reconnection, turbulence, waves, jets and so on. All these processes are related to dynamical evolving plasma structures in both space and time. In this context, invariant quantities derived from the gradient tensor method allows us to study the evolution of topological structures in velocity and magnetic fields across various regions of interplanetary space at different scales. The use of gradient tensors is primarily based on the availability of multi-point data from missions involving at least four satellites arranged in a tetrahedral formation.

Here we present some theoretical and observational results based on the analysis of gradient tensor invariants. We derive equations governing the temporal evolution of these quantities to get insights into the topological and morphological changes of these structures in time. These evolution equations also allow us to identify the dominant physical terms driving the observed changes. A preliminary analysis, based on MMS multi-point observations, suggests that the plasma in the near-Earth solar wind predominantly behaves like a fluid, whereas velocity and magnetic field interactions play a more significant role in the magnetosheath region.
We further introduce a novel approach for studying gradient tensor characteristics using the Schur transformation. This technique decomposes the velocity and magnetic field gradient tensors into a matrix representing eigenvalue contributions and another term associated with pressure and dissipative effects. This decomposition enables the identification of regions where dissipative effects are more prominent. These studies are of critical importance for future space missions which will extend the current multi-point paradigm, based on a single tetrahedron constellation, to multi-scale multiple tetrahedra configurations such as the NASA mission HelioSwarm (in the solar wind) and the ESA Phase A Plasma Observatory (in the near-Earth plasma).

How to cite: Quattrociocchi, V., Consolini, G., Materassi, M., and Benella, S.: Investigating structures through gradient tensors in turbulent space plasmas: invariants’ evolution equations and Schur decomposition, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17806, https://doi.org/10.5194/egusphere-egu25-17806, 2025.

EGU25-17870 | Posters on site | ST2.8

The ESA M7 Plasma Observatory mission 

Maria Federica Marcucci and Alessandro Retinò and the The Plasma Observatory Team

The Magnetospheric System is the highly dynamic plasma environment where the strongest energization and energy transport occurs in near-Earth space.  Previous multi-point observations from missions such as ESA/Cluster and NASA/MMS have evidenced the fundamental role for these processes of cross-scales coupling . In the Magnetospheric System, the electromagnetic energy is converted into energized particles and energy is transported mainly at the ion and fluid scales. Simultaneous measurements at both large, fluid and small, kinetic scales are required to resolve scale coupling and ultimately fully understand plasma energization and energy transport processes. Here, we present the Plasma Observatory (PO) multi-scale mission concept tailored to study plasma energization and energy transport in the Earth's Magnetospheric System through with the first simultaneous in situ measurements at both fluid and ion scales. PO baseline mission includes one mothercraft (MSC) and six identical smallsat daughtercraft (DSC) in a two tetrahedra formation with MSC at the common vertex for both tetrahedra. PO baseline orbit is an HEO 8x17 RE orbit, covering all the key regions of the Magnetospheric System including the foreshock, the bow shock, the magnetosheath, the magnetopause, the transition region and the current sheet. Spacecraft separation ranges from fluid (5000 km) to ion (30 km) scales. The MSC payload provides a complete characterization of electromagnetic fields and particles in a single point with time resolution sufficient to resolve kinetic physics at sub-ion scales and fully characterize wave-particle interactions. The DSCs have identical payload, simpler than the MSC payload, yet giving a full characterization of the plasma at the ion and fluid scales and providing the context where energization and transport occurs. PO is the next logical step after Cluster and MMS and will allow us to resolve for the first time scale coupling in  the Earth's Magnetospheric System, leading to transformative advances in the field of space plasma physics. Plasma Observatory  is one of the three ESA M7 candidates, which have been selected in November 2023 for a competitive Phase A with a mission selection planned in 2026 and launch in 2037.  

How to cite: Marcucci, M. F. and Retinò, A. and the The Plasma Observatory Team: The ESA M7 Plasma Observatory mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17870, https://doi.org/10.5194/egusphere-egu25-17870, 2025.

EGU25-17894 | Posters on site | ST2.8

The MAG-M magnetometer onboard Plasma Observatory 

Lorenzo Matteini, Patrick Brown, Madeleine Tomes, and John Hodgkins

Plasma Observatory (PO) is an ESA mission proposal to study for the first time plasma transport and energization in the near-Earth environment simultaneously at both fluid and ion scales, with a constellation of 7 spacecraft: 1 mother and 6 daughters. 
In the PO mission framework, MAG-M is the proposed fluxgate magnetometer onboard the Mothercraft, to be built at Imperial College London.
It is a dual-sensor instrument mounted on a rigid boom dedicated to high-resolution measurements of the DC magnetic field, with strong design heritage from previous missions. In this presentation we review MAG-M main characteristics and its development stage. 
We also discuss the key role of magnetic field measurements in the goals of the mission and how MAG-M will contribute, both with single-point and multi-point measurements, to the investigation of the nature of waves and structures in the plasma at both fluid and kinetic scales, their vector anisotropies, the 3-dimensional shapes of eddies and boundaries in the plasma as well as to the determination of the flows of energy acting between particles and fields in the near-Earth environment.

How to cite: Matteini, L., Brown, P., Tomes, M., and Hodgkins, J.: The MAG-M magnetometer onboard Plasma Observatory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17894, https://doi.org/10.5194/egusphere-egu25-17894, 2025.

Understanding the turbulence of collisionless space plasmas is one a major open frontiers towards the disclosure of the mechanisms of energization of the plasmas of the Universe, the acceleration of particles and bulk plasma flows, the heating of the plasma.

The interacting plasma particles and multiscale modes of the plasma turbulence form a system of complex nonlinear interactions which cannot be described analytically.

Instead, their behavior is investigated statistically, by means of kinetic numerical simulations.

We report the current state of the art of these simulations which revealed the important role of the electrons even for larger (ion-) scale processes in the collisionless turbulence.

Based on those new results we derive the necessity and parameters of future multispacecraft investigations of spectra and structure formation processes in turbulent space plasmas beyond the results obtained by CLUSTER and MMS observations.

How to cite: Büchner, J.: Need of multispacecraft observations to understand collisionless turbulent solar system plasmas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17916, https://doi.org/10.5194/egusphere-egu25-17916, 2025.

EGU25-17978 | Orals | ST2.8

An Electron Plasma Camera for the Plasma Observatory ESA mission 

Matthieu Berthomier, Colin Forsyth, Frédéric Leblanc, Jean-Denis Techer, Yvon Alata, Gabriel Poggia, Evan Seneret, Chris Brockley-Blatt, Alessandro Retino, and Olivier Le Contel

Measuring both the energy spectrum and the 3D distribution of charged particles at high temporal resolution is one of the main challenges in space plasma instrumentation. The conventional solution to date has been to use multiple sensors that couple the native quasi-2D instantaneous field of view of the electrostatic top-hat analyser with a scanning electrostatic deflection system.

For the Plasma Observatory ESA mission, we proposed an alternate strategy that reduces the level of resources required for rapid plasma measurements at sub-ion scale in the magnetospheric environment. The Electron Plasma Camera (EPC) is based on the donut-shaped electrostatic analyser topology that do not require any electrostatic scanning to provide a hemispheric field-of-view of the surrounding plasma.

This optics is manufactured through the selective metallization of a high-resolution 3D printed polymer. It is coupled to a 256-pixel imaging detection system that uses the detection technology that was demonstrated on the Solar Orbiter mission.  EPC’s fully integrated front-end electronics takes advantage of the high-geometric factor of its electrostatic optics to enable the capture of high temporal resolution images of electron phase space. We present the expected capability of the instrument in the key science regions the Plasma Observatory mission will encounter, and some of the major science questions related to multi-scale phenomena the Plasma Observatory mission will address with its unique data set.

How to cite: Berthomier, M., Forsyth, C., Leblanc, F., Techer, J.-D., Alata, Y., Poggia, G., Seneret, E., Brockley-Blatt, C., Retino, A., and Le Contel, O.: An Electron Plasma Camera for the Plasma Observatory ESA mission, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17978, https://doi.org/10.5194/egusphere-egu25-17978, 2025.

EGU25-18438 | ECS | Posters on site | ST2.8

2D fully kinetic simulations of dayside magnetic reconnection in the presence of cold ions and a moderate guide field. 

Mohammed Baraka, Olivier Le Contel, Alessandro Retino, Jérémy Dargent, Arnaud Beck, Sergio Toledo-Redondo, Giulia Cozzani, Stephen Fuselier, Thomas Chust, and Soboh Alqeeq

The standard conditions considered for magnetic reconnection to occur are usually antiparallel magnetic field configurations with a shear angle of 180. Reconnection is often observed with an additional out-of-plane component of the magnetic field (guide field). We performed two sets of 2D fully kinetic simulations using SMILEI code of asymmetric reconnection. The first set was performed initially by Dargent et al., 2017 with and without cold ions. While the second set with and without cold ions each conducted in the presence of a moderate guide field. The simulation domain size is set to (xmax , ymax) = (320, 128) di, enabling us to study these effects in the electron diffusion region (EDR) as well as the coupling across different scales, including ion diffusion region (IDR), outflow jets, and extended separatrices far from diffusion region. When the density gradient is combined with a guide field component at the magnetopause, it was suggested by Swisdak et al., 2003 that the electron diamagnetic drift governs the motion of the X-line.

Our simulations reveal the development of an asymmetry in the reconnection plane as expected and a motion of the X-line in the opposite direction of the electron diamagnetic drift. This finding challenges the previously proposed explanation. We also report our progress in investigating the impact of cold ions in reinforcing the electron dynamics and further investigate the impact of adding a moderate guide field in their presence. These effects are expected to influence the energization, energy partitioning across scales, and potentially the suppression of reconnection. Fluid scales coupling with smaller ion scales aligns with the primary objective of the Plasma Observatory (PO) mission which aims to study plasma energization and energy transport. Our findings will contribute to the preparation of the PO mission and aim at improving its science return.

How to cite: Baraka, M., Le Contel, O., Retino, A., Dargent, J., Beck, A., Toledo-Redondo, S., Cozzani, G., Fuselier, S., Chust, T., and Alqeeq, S.: 2D fully kinetic simulations of dayside magnetic reconnection in the presence of cold ions and a moderate guide field., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18438, https://doi.org/10.5194/egusphere-egu25-18438, 2025.

EGU25-18777 | Posters on site | ST2.8

The Particle Processing Unit (PPU-M) on-board the Plasma Observatory Mother Spacecraft 

Edoardo Rota, Raffaella D'Amicis, Maria Federica Marcucci, Rossana De Marco, Rosanna Rispoli, Matthieu Berthomier, Robert Wimmer-Schweingruber, and Francesco Valentini

Plasma Observatory (PMO) is a candidate for the ESA Directorate of Science M7 mission call, currently in Phase A. It is a multi-scale mission concept with the capability to resolve scale coupling and non-planarity/non-stationarity in plasma energization and energy transport.

On board the mothercraft, the Particle Processing Unit (PPU-M) will be the single interface between the spacecraft and all the particle instruments: the Electron Particle Chamber (EPC-M), the Ion Mass Spectrometer (IMS) and the Energetic Particle Experiment (EPE-M). The PPU-M provides a single power, telemetry, and control interface to the spacecraft as well as power switching, commanding and data handling for the particle instruments. The PPU-M will have a fully redundant configuration, with two CPU boards (nominal and redundant), based on the dual-core LEON3FT processor and two groups of 3 Compression and Scientific Processing (CSP) boards based on FPGAs.

The approach of a common data processing unit for all the particle instruments allows to efficiently handle the data rate from all the particle instruments and the data processing on board, also facilitating interoperation with the other instruments on the spacecraft. Moreover, it allows technical and programmatic synergies giving the possibility to optimize and save spacecraft resources. Here, we will describe the PPU-M characteristics and functionalities.

How to cite: Rota, E., D'Amicis, R., Marcucci, M. F., De Marco, R., Rispoli, R., Berthomier, M., Wimmer-Schweingruber, R., and Valentini, F.: The Particle Processing Unit (PPU-M) on-board the Plasma Observatory Mother Spacecraft, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18777, https://doi.org/10.5194/egusphere-egu25-18777, 2025.

EGU25-19084 | Posters on site | ST2.8

The Plasma Observatory FIELDS-M instrument suite 

Andrew Dimmock, Yuri Khotyaintsev, Vicki Cripps, Lorenzo Matteini, Olivier Le Contell, Matthieu Kretzschmar, Stuart Bale, Hanna Rothkaehl, Jan Soucek, Lea Griton, Karine Issautier, Nicholay Ivchenko, and Marek Morawski

The Plasma Observatory mission aims to advance our understanding of fundamental plasma processes, including energy transfer, turbulence, and reconnection, by deploying a constellation of seven spacecraft: one "Mother" craft and six smaller "Daughter" craft.

The FIELDS-M instrument suite, part of the  "Mother" craft payload, is designed to provide comprehensive measurements of electric and magnetic fields, plasma waves, necessary to characterize wave-particle interactions in Earth's magnetosphere and beyond. 

FIELDS-M is a collaborative effort, integrating multiple sensors and electronics to measure electric fields, magnetic fields, and wave spectra over a broad frequency range. The instrument suite consists of electric field probes, search-coil magnetometers, fluxgate magnetometers, and wave analyzers, enabling high-resolution observations of both large-scale and microphysical plasma dynamics. 

How to cite: Dimmock, A., Khotyaintsev, Y., Cripps, V., Matteini, L., Le Contell, O., Kretzschmar, M., Bale, S., Rothkaehl, H., Soucek, J., Griton, L., Issautier, K., Ivchenko, N., and Morawski, M.: The Plasma Observatory FIELDS-M instrument suite, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19084, https://doi.org/10.5194/egusphere-egu25-19084, 2025.

EGU25-19099 | Orals | ST2.8

Non-stationarity, ion reflection, and wave-particle interactions at quasi-perpendicular shocks 

Yuri Khotyaintsev, Daniel Graham, Domenico Trotta, Ahmad Lalti, Andrew Dimmock, and Mengmeng Wang

Quasi-perpendicular collisionless shocks are fundamental structures in space plasmas, where the absence of collisions necessitates electromagnetic fields to mediate energy dissipation and particle dynamics. The Magnetospheric Multiscale (MMS) mission, with its high-resolution measurements and multi-point capabilities, provides unique insights into these complex processes. We present MMS observations of ion reflection, electron and ion heating, non-stationarity, wave-particle interactions at quasi-perpendicular shocks. Ion reflection is observed as a critical mechanism for energy transfer, contributing to downstream heating and the generation of instabilities. Non-stationary shock structures, such as ripples and reformation, are identified, showcasing dynamic variations in shock parameters over short spatial and temporal scales. Wave-particle interactions are examined in detail, revealing the role of reflected and minor ions in driving electrostatic and electromagnetic wave activity near the shock front. The observations highlight the interplay between reflected ions and wave generation, which collectively govern shock dynamics and determine the downstream plasma properties. We discuss the need for the novel fields and particle measurements to be provided by Plasma Observatory in order to address the remaining open questions in the field.

How to cite: Khotyaintsev, Y., Graham, D., Trotta, D., Lalti, A., Dimmock, A., and Wang, M.: Non-stationarity, ion reflection, and wave-particle interactions at quasi-perpendicular shocks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19099, https://doi.org/10.5194/egusphere-egu25-19099, 2025.

EGU25-19321 | ECS | Posters on site | ST2.8

Plasma Observatory’s Group on sImulAtioN NumerIcal support (GIANNI) 

Markku Alho, Domenico Trotta, and Francesco Valentini and the Plasma Observatory's Group on sImulAtioN NumerIcal support (GIANNI)

The ESA M7 mission candidate Plasma Observatory proposal’s Group on sImulAtioN NumerIcal support (GIANNI) is tasked with supporting the proposal's Science Study Team with simulation data, to help evaluate the proposal's science impact, assess possible descoping options and their effects on science output, and provide constraints for the PO constellation parameters.

In this presentation, we summarize the composition and capabilities of the group and the represented simulation models. This includes collating a  repository of tools and short manuals and tutorials for the sorts of simulation datasets available and their possible use cases, and how to work with us to set up virtual observatories in the varied numerical models. We present an overview of the group's science support activities.

How to cite: Alho, M., Trotta, D., and Valentini, F. and the Plasma Observatory's Group on sImulAtioN NumerIcal support (GIANNI): Plasma Observatory’s Group on sImulAtioN NumerIcal support (GIANNI), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19321, https://doi.org/10.5194/egusphere-egu25-19321, 2025.

EGU25-21857 | Posters on site | ST2.8

US Contributions to the Plasma Observatory Mission  

Lynn M. Kistler, Harald Kucharek, Vassilis Angelopoulos, Stuart. D. Bale, John Bonnell, Malcolm Dunlop, Yuri Khotyaintsev, Alessandro Retinò, and Maria Federica Marcucci

Plasma Observatory (PO) is a Heliophysics mission that will explore plasma energization and energy transport in the Earth’s Magnetospheric System, for the first time through multi-scale observations covering simultaneously the ion and fluid scales. PO is currently in a competitive ESA Phase A study as one of the three candidates for the future ESA M7 mission. From its  equatorial, 8 by 18 RE (geocentric perigee and apogee, respectively, in Earth radii), 15o inclination orbit, PO will  addresses the following science questions: (Q1) how particles are energized in space plasmas and (Q2) which processes dominate energy transport and drive coupling across regions of Earth’s magnetosphere. The aforementioned science questions being pursued by PO are aligned with the goals of NASA’s SMD3,4: to understand the physical processes, and Sun-Earth connections. The PO baseline mission will achieve this objective with a comprehensively instrumented mother spacecraft (MSC) or mothercraft, and six identical smallsat daughtercraft (DSC). After highly successful missions such as Cluster, Themis, and MMS, this will be the next logical step to gain transformative insights into fundamental processes of the Magnetospheric System.

 

A team of US scientists from three major institutions will provide significant parts of three instruments for the P.O. payload.  UNH (University of New Hampshire) will provide the time-of-flight and detector section and some electronics for the Ion Mass Spectrometer (IMS-M) that will measure the 3D distributions of (H+ , He+ , He++ and O+ ) at high time resolution. This ion spectrometer will be placed on the mothercraft. The University of Berkeley (UCB) will provide  the spin-plane double-probe electric field sensors of the electric field instrument EFI-M onboard the mothercraft,  based on the ones flown on RBSP. The University of California in Los Angeles will be providing the mechanical design of the detectors, telescopes and electronics box, and the design of the power and digital processing electronics boards for the energetic particle instrument EPE-D on each of the six daughtercraft, based on heritage from the ELFIN mission.  These contributions are critical for the success of the PO mission and its science return. The US team is currently collaborating with the PO consortium in the ESAPhase A study to determine how to efficiently provide the payload that will return the best quantity measurements.  In this presentation we will introduce the capability of these instruments and the current achievements and progress that were obtained during the ongoing phase A study.

How to cite: Kistler, L. M., Kucharek, H., Angelopoulos, V., Bale, S. D., Bonnell, J., Dunlop, M., Khotyaintsev, Y., Retinò, A., and Marcucci, M. F.: US Contributions to the Plasma Observatory Mission , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21857, https://doi.org/10.5194/egusphere-egu25-21857, 2025.

EGU25-21888 | ECS | Posters on site | ST2.8

 The Plasma Observatory Ground-Based Coordination Working Group  

Jonathan Rae and the Plasma Observatory Ground-Based Coordination Working Group

Plasma Observatory is one of three “M-class” missions that are going through Phase A studyAn unprecedented seven spacecraft mission to understand plasma energisation across both ion and fluid scales, Plasma Observatory will bring step-change understanding in how particles are accelerated in astrophysical plasmasIn order to gain the best possible scientific breakthroughs, it is essential that collaboration and coordination with ground-based instruments and facilities occurs as quickly as possibleHere we discuss the scientific and practical aspects of ground-based facilities and the synergies with Plasma Observatory across all of the mission profileWe also seek to recruit more interested participants in the ground-based working group through the Phase A process and beyond. 

How to cite: Rae, J. and the Plasma Observatory Ground-Based Coordination Working Group:  The Plasma Observatory Ground-Based Coordination Working Group , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21888, https://doi.org/10.5194/egusphere-egu25-21888, 2025.

EGU25-118 | ECS | Orals | CR2.2

To what extent is climate change responsible for retreat of the Pine Island Glacier over the 20th century? 

Alex Bradley, David Bett, Paul Holland, Rob Arthern, and Rosie Williams

The relative contributions of anthropogenic climate change and internal variability in sea level rise from the Antarctic Ice Sheet are yet to be determined. This is primarily because of uncertainty arising from poorly constrained model parameters and chaotic forcing as well as a relatively short observation period. Using an established uncertainty quantification framework (known as calibrate-emulate-sample), we have quantified, for the first time, the role of anthropogenic climate change on retreat of a major Antarctic glacier. We find that anthropogenic trends in forcing, beginning in the 1960s, are only responsible for approximately 15% of the retreat of this glacier since its retreat began in the 1940s. Most of the retreat is attributable to the inertia associated with a slow retreat over the Holocene. We also find, however, that trends in forcing dominate retreat beyond the 21st century, with ice sheet retreat stabilized if anthropogenic trends plateau.

How to cite: Bradley, A., Bett, D., Holland, P., Arthern, R., and Williams, R.: To what extent is climate change responsible for retreat of the Pine Island Glacier over the 20th century?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-118, https://doi.org/10.5194/egusphere-egu25-118, 2025.

EGU25-332 | ECS | Posters on site | CR2.2

Links between GRACE/GRACE-FO derived temporal mass variations in Greenland and climatic indices 

Florent Cambier, José Darrozes, Muriel Llubes, Lucia Seoane, and Guillaume Ramillien

The Greenland Ice Sheet (GIS) has been experiencing significant mass loss since the 1990s, driven by the intensifying effects of global warming. However, this global trend is modulated by distinct annual and interannual variations, highlighting the complex interplay between the ice sheet, atmospheric systems, and the ocean. In this study, we analyzed GIS mass changes from early 2002 to late 2023 using data from the GRACE and GRACE-FO missions, focusing on the dominant temporal cycles and their relationships with climatic indices and parameters.

Using Empirical Orthogonal Functions (EOF) applied to mass variation data from the COST-G solution, we identified five leading modes of variability, accounting for 67.5% of the total variance. The primary mode capture both the annual cycle and longer-term periodicities, while subsequent modes highlight interannual oscillations, with cycles ranging from 4 to 11 years.

We examined the interactions between GIS mass changes and six key climatic drivers: the North Atlantic Oscillation (NAO), Greenland Blocking Index (GBI), Atlantic Multidecadal Oscillation (AMO), temperature duration and intensity, precipitation, and surface albedo. Cumulative indices and parameters enabled direct comparisons with the accumulated mass changes since 2002. Through Wavelet Analysis and cross-correlations, we uncovered significant links with varying time lags. They lead to a complete annual cycle and some interannual relationship between them. For instance, a positive NAO phase enhances precipitation, while the AMO displays a surprising 3.5-year delayed response to mass variations.

Additionally, our findings reveal a connection between 11-year cycles in NAO, GBI, and temperature to solar activity, while 4 to 7-year cycles align with potential atmospheric oscillations and Earth’s internal geodynamics.

This study highlights the GIS as a dynamic system modulated by interrelated processes operating on annual to decadal timescales. We have only investigated Greenland in its globality, but we know that the response to external forcing at a scale of a basin or a glacier differs. It will be important to examine this point as the integrations of multi-scale climatic drivers is important to understand past variations and project future changes under a warming climate. Such understanding is vital for assessing global sea-level rise and formulating mitigation strategies.

How to cite: Cambier, F., Darrozes, J., Llubes, M., Seoane, L., and Ramillien, G.: Links between GRACE/GRACE-FO derived temporal mass variations in Greenland and climatic indices, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-332, https://doi.org/10.5194/egusphere-egu25-332, 2025.

The Marine Isotope Stage (MIS) 12-MIS 11 glacial cycle (490-396 Ka) has been recognized as anomalous by researchers due to the longevity of the interglacial interval.  MIS 12 sea level low stand is inferred to be similar to Last Glacial Maximum (LGM), however, due to limited geomorphological data, major uncertainties remain with respect to where the ice was distributed and the relative size of the ice sheets. With the lowest increase in insolation from glacial to interglacial of the past 800 kyrs, MIS 11 was almost twice as long as the other interglacials of the past 500 kyrs. A prevailing hypothesis for the duration of MIS 11 proposes that the large MIS 12 ice sheets, when exposed to a weak insolation increase, gradually released meltwater and deglaciated throughout the interglacial period, contributing to its extended duration. This freshwater influx triggered a positive feedback, promoting the release of oceanic CO2 into the atmosphere, which amplified insolation-driven warming and further prolonged the interglacial period.

Given the lack of terrestrial paleoclimate data, ice and climate modelling may offer a way to improve the understanding of this curious interval. Previous modeling work of this interval has been with either highly parameterized, low-resolution coupled ice-climate models, climate models with forced ice sheets, snapshot climate models with pre-industrial ice sheets, or ice sheet models with forced climate. Few models span the entire duration of the glacial cycle. For the first time, we transiently simulate the entire interval with the fully coupled ice sheet-climate LCIce model that resolves both atmospheric and ocean circulation. Parametric uncertainties are addressed by ensemble simulation. This presentation focuses on ensemble analysis of the ice sheets and climate of the glacial cycle as well as sensitivity testing of the two hypothesized drivers for length of MIS 11: meltwater flux during deglaciation and atmospheric CO2 concentration.

How to cite: Parnell, A. and Tarasov, L.: Ensemble simulation of the MIS 12-MIS 11 glacial cycle using a fully coupled climate-ice sheet model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-577, https://doi.org/10.5194/egusphere-egu25-577, 2025.

EGU25-1396 | ECS | Orals | CR2.2

Modeled Greenland Ice Sheet evolution constrained by ice-core-derived Holocene elevation histories 

Mikkel Langgaard Lauritzen, Anne Munck Solgaard, Nicholas Mossor Rathmann, Bo Møllesøe Vinther, Aslak Grindsted, Brice Noël, Guðfinna Aðalgeirsdóttir, and Christine Schøtt Hvidberg

During the Holocene, the Greenland Ice Sheet (GrIS) experienced substantial thinning, with some regions losing up to 600 meters of ice.
Ice sheet reconstructions, paleoclimatic records, and geological evidence indicate that during the Last Glacial Maximum, the GrIS extended far beyond its current boundaries and was connected with the Innuitian Ice Sheet (IIS) in the northwest. We investigate these long-term geometry changes and explore several possible factors driving those changes by using the Parallel Ice Sheet Model (PISM) to simulate the GrIS thinning throughout the Holocene period, from 11.7 ka ago to the present. We perform an ensemble study of 841 model simulations in which key model parameters are systematically varied to determine the parameter values that, with quantified uncertainties, best reproduce the 11.7 ka of surface elevation records derived from ice cores, providing confidence in the modeled GrIS historical evolution. We find that since the Holocene onset, 11.7 ka ago, the GrIS mass loss has contributed 5.3±0.3 m to the mean global sea level rise, which is consistent with the ice-core-derived thinning curves spanning the time when the GrIS and the Innuitian Ice Sheet were bridged. Our results suggest that the ice bridge collapsed 4.9±0.5 ka ago and that the GrIS is still responding to these past changes today. Our results have implications for future mass-loss projections, which should account for the long-term, transient trend.

How to cite: Lauritzen, M. L., Solgaard, A. M., Rathmann, N. M., Vinther, B. M., Grindsted, A., Noël, B., Aðalgeirsdóttir, G., and Hvidberg, C. S.: Modeled Greenland Ice Sheet evolution constrained by ice-core-derived Holocene elevation histories, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1396, https://doi.org/10.5194/egusphere-egu25-1396, 2025.

EGU25-3494 | ECS | Orals | CR2.2

Constraining the extent of the Greenland Ice Sheet during warmer climates of the Pliocene and Pleistocene: insights from subglacial geomorphology 

Guy Paxman, Stewart Jamieson, Kirsty Tinto, Jacqueline Austermann, Aisling Dolan, and Mike Bentley

The Greenland Ice Sheet is a key contributor to contemporary global sea-level rise, but its long-term history remains highly uncertain. The landscape covered by the ice sheet comprises ∼79% of Greenland and is one of the most sparsely mapped regions on Earth. However, sub-ice geomorphology offers a unique record of environmental conditions prior to and during glaciation, and of the ice sheet’s response to changing climate.

Here we use ice-surface morphology and radio-echo sounding data to identify, and quantify the morphology of, valley networks beneath the Greenland Ice Sheet. Our mapping reveals intricate subglacial valley networks beneath the ice-sheet interior that appear to have a fluvial origin. By contrast, in the southern and eastern coastal highlands, valleys have been substantially modified by glacial erosion. We use geomorphometric analysis and simple ice-sheet model experiments to infer that these valleys were incised beneath erosive mountain valley glaciers during one or more phases of Greenland’s glacial history when ice was restricted to the southern and eastern highlands.

These inferred early mountain ice masses contained ~0.5 metres of sea-level equivalent (compared to 7.4 metres in the modern Greenland Ice Sheet). We believe the most plausible time for the formation of this landscape was prior to the growth of a continental-scale ice sheet in the late Pliocene, with the possibility of further incision having occurred during particularly warm and/or long-lived Pleistocene interglacials. Our findings therefore provide new data-based constraints on early Greenland Ice Sheet extent and dynamics that can serve as valuable boundary conditions in models of regional and global palaeoclimate during past warm periods that are important analogues for climate change in the 21st century and beyond.

How to cite: Paxman, G., Jamieson, S., Tinto, K., Austermann, J., Dolan, A., and Bentley, M.: Constraining the extent of the Greenland Ice Sheet during warmer climates of the Pliocene and Pleistocene: insights from subglacial geomorphology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3494, https://doi.org/10.5194/egusphere-egu25-3494, 2025.

EGU25-4341 | ECS | Orals | CR2.2

Ice sheet-ocean interactions at 40 kyr BP : Insights from a coupled ice sheet-climate model of intermediate complexity. 

Louise Abot, Aurélien Quiquet, and Claire Waelbroeck

This study examines the interactions between the Northern Hemisphere ice sheets and the ocean during the last glacial period. Using the iLOVECLIM climate model of intermediate complexity coupled with the GRISLI ice sheet model, we explore the consequences of an amplification of the melt rates beneath ice shelves on ice sheet dynamics and the associated feedbacks. First, the amplification of oceanic basal melt rates leads to significant freshwater release from both increased calving and basal melt fluxes. Grounding line retreat and dynamic thinning occur over the Eurasian and Iceland ice sheets, while the oceanic perturbation fails to trigger a grounding line migration over the coasts of Greenland and the eastern part of the Laurentide ice sheet. Second, similarly to hosing experiments with no coupling between the climate and the ice sheets, the influx of fresh water temporarily increases sea-ice extent, reduces convection in the Labrador Sea, weakens the Atlantic meridional overturning circulation, lowers surface temperatures in the Northern Hemisphere, and increases the subsurface temperatures in the Nordic Seas. Third, the freshwater release and latent heat effect on ocean temperatures lead to a decrease in ice sheet discharge (negative feedback) for the Greenland and Eurasian ice sheets. In the experiments, the Laurentide ice sheet does not feature significant volume variations. Nonetheless, we show that we are able to trigger a grounding line retreat and a North American ice sheet volume decrease, by imposing ad-hoc constant oceanic melt rates in a second set of perturbation experiments. However, the Hudson Strait ice stream also does not exhibit the past dynamical instability indicated by the presence of Laurentide origin ice rafted debris in the North Atlantic sediment records.  This suggests that the fully coupled model is too stable, specifically in the Hudson Bay region. To help address this issue, different modelling choices regarding the basal ice sheet dynamics are considered. This emphasizes the need for further research using fully coupled models to explore the triggering mechanisms of massive iceberg discharges and to clarify the role of the ocean in these events.

How to cite: Abot, L., Quiquet, A., and Waelbroeck, C.: Ice sheet-ocean interactions at 40 kyr BP : Insights from a coupled ice sheet-climate model of intermediate complexity., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4341, https://doi.org/10.5194/egusphere-egu25-4341, 2025.

EGU25-4663 | ECS | Orals | CR2.2

Greenland Ice Sheet under climate change: Perspective from a high-resolution modelling simulation from 1421-2024   

Aaquib Javed, Edward Hanna, Leanne Wake, Richard Wilkinson, Mathieu Morlighem, and Joe Mcconnell

The Greenland Ice Sheet (GrIS), a major driver of global sea-level rise, holds approximately 7 meters of sea-level equivalent. Despite its critical role, significant uncertainties remain about its mass balance and response to climate forcing over the past few centuries, particularly before the satellite era. This study aims to address these gaps by reconstructing a high-resolution (1x1 km) monthly surface mass balance (SMB) dataset spanning AD 1421–2024 and quantifying its contributions to historical and contemporary sea-level changes using the Positive Degree Day (PDD) modelling approach. 

The novel SMB dataset integrates long-term climate reanalysis inputs (ERA5 and ModE-RA). They are then validated and corrected against available ice-core records and weather station observations using a Bayesian approach to formally constrain the uncertainties. Preliminary analysis indicates signidficant SMB-driven mass loss due to climatic forcing during recent past, potentially offering new insights into the relative contributions of SMB and ice dynamics to GrIS total mass changes during latter half of the last millennium. 

These results represent a significant advancement in understanding the GrIS’s historical behaviour and links with climate change and can form a valuable baseline for improving the accuracy of future SMB and sea-level rise projections. By addressing critical knowledge gaps, this work enhances our ability to predict the long-term impacts of climate change on the GrIS and global sea levels.

How to cite: Javed, A., Hanna, E., Wake, L., Wilkinson, R., Morlighem, M., and Mcconnell, J.: Greenland Ice Sheet under climate change: Perspective from a high-resolution modelling simulation from 1421-2024  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4663, https://doi.org/10.5194/egusphere-egu25-4663, 2025.

EGU25-5578 | ECS | Posters on site | CR2.2

Snow accumulation rates at Concordia Station from stake farm observations 

Claudio Stefanini, Barbara Stenni, Mauro Masiol, Giuliano Dreossi, Massimo Frezzotti, Vincent Favier, Francesca Becherini, Claudio Scarchilli, Virginia Ciardini, and Gabriele Carugati

In this study, surface mass balance (SMB) is estimated from snow accumulation data collected in the nearby area of Concordia Station. Results from the Italian and French stake farms are jointly analyzed. The Italian stake farm is located ~800 m southwest of the Concordia Station and consists of 13 stakes; observations started at the end of 2010 with almost monthly sampling. Some measurements are also available for the 2006-2010 period from a previous stake farm which was located ~300 m east of the current site. The French stake farm is located ~2 km south of the base and consists of 50 stakes; observations started in 2004 with yearly sampling conducted during austral summer. Snow build-up measurements at individual stakes show a strong variability caused by the interaction of wind-driven snow with surface micro-relief. Over the period of common observations, the present Italian stake farm generally underestimates the snow accumulation with respect to the French one, except for three years in which an overestimation is observed. Over the 2011-2023 period, the mean yearly accumulation recorded by the Italian and French stake farms is 7.3±0.2 cm and 8.4±0.1 cm, respectively. Bootstrap simulation has been performed to: (i) assess the significance of the differences between the two datasets; (ii) evaluate the effect of the different size of the stake farms and their distance to the Station on the measurements. Comparison of the observations with reanalysis datasets (ERA5 and MERRA2) and regional models (RACMO, MAR) has been also performed, with the first ones providing the best agreement with the observations. The potential shadowing effect of the station has also been investigated by analyzing the wind direction during the snowfall events, suggesting that buildings may influence accumulation when they are upwind with respect to the stake farms. Additionally, two more stake farms, located 25 km north and south of Concordia Station, are also analyzed to study the accumulation gradient across Dome C, confirming previous results of a continentality effect. On average, yearly accumulation increases by 0.7±0.2 cm over the 50 km span between the southern and northern stake farms. Results should be valuable for validating SMB estimates obtained from reanalysis, regional climate models and remote-sensing data.

How to cite: Stefanini, C., Stenni, B., Masiol, M., Dreossi, G., Frezzotti, M., Favier, V., Becherini, F., Scarchilli, C., Ciardini, V., and Carugati, G.: Snow accumulation rates at Concordia Station from stake farm observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5578, https://doi.org/10.5194/egusphere-egu25-5578, 2025.

The importance of employing a two-way coupled climate-ice sheet model for future sea level projection has been revealed by LOVECLIP simulation. However, it still has several limitations. LOVECLIM, the climate model used in LOVECLIP, is unsuitable for short-term simulation. Additionally, LOVECLIM with a low-resolution T21 cannot solve regional-scale changes over the Antarctic region. Therefore, we newly coupled CESM1.2 to the Penn State Ice Sheet Model (PSUIM). CESM1.2 consists of the Community Atmosphere Model (CAM) with a f09 resolution for the atmosphere and Parallel Ocean Program version 2 (POP2) with a gx1v6 resolution for the ocean. Using coupled CESM1.2-PSUIM, we projected the responses of Greenland and Antarctic ice sheets, as well as future climate and sea level rise under the Representative Concentration Pathway scenarios.

How to cite: Park, J.: Coupled CESM1.2 to Penn State University Ice Sheet Model and future sea level projection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6338, https://doi.org/10.5194/egusphere-egu25-6338, 2025.

EGU25-6677 | ECS | Orals | CR2.2

A combined radiostratigraphy- and ice-core- derived age scale for ice at the divide between the Amundsen, Bellingshausen and Weddell seas, West Antarctica 

Harry Davis, Robert Bingham, Andrew Hein, Anna Hogg, Carlos Martín, and Elizabeth Thomas

Despite ice cores providing high-resolution climate records, few ice cores extracted from the West Antarctic Ice Sheet (WAIS) cover the Holocene, nor extend into the last glacial period. Marine ice-sheet basins, such as those underlying the WAIS, have been shown to be particularly vulnerable to retreat and possible collapse during past warm periods, and thus have significant potential to contribute to global sea-level rise. Dynamic thinning and retreat of ice are underway in the Amundsen Sea and Bellingshausen Sea sectors of the WAIS, yet this Pacific-facing region remains relatively data-poor for informing estimates of past and future retreat rates and sea-level contributions.

In 2010/11, a 136 m ice core was drilled at the three-way ice divide between Ferrigno Ice Stream, Pine Island Glacier, and Evans Ice Stream catchments. To further investigate this region, we analyse the internal structure across this region imaged through three intersecting radar surveys: (1) a 2004/05 UK/BAS survey, conducted with the Polarimetric Airborne Survey INstrument (PASIN), (2) a 2009/10 ground-based survey of Ferrigno Ice Stream, carried out with 3 MHz radar; and (3) NASA Operation Ice Bridge airborne surveys acquired in 2016 and 2018, which utilised the Multichannel Coherent Radar Depth Sounder 2 (MCoRDS2). We provide dating control to the traced englacial stratigraphy from tying it to the age-depth profile provided by the WAIS Divide Ice Core in central West Antarctica.

We then utilise a 1-D numerical ice-flow model, optimised by shallow ice-core data and these dated internal reflection horizons at the three-way ice divide, to infer palaeo-accumulation rates throughout the Holocene, and place age constraints on the age of the oldest ice at a proposed deep ice-core drill site at Ferrigno Ice Stream. We show that the method is robust and effectively synthesises the shallow ice-core data and the dated internal reflection horizons to reconstruct past climate records. The modelled maximum age at the three-way ice divide is around 24.77 ka +/- 6.88 ka, with a resolution of around 0.6 ka m-1at the depth of the oldest ice, making this an ideal site for a new deep ice core in West Antarctica. In addition, the ice core would be located in a coastal area and may provide key insights glacial extent during deglaciation.

How to cite: Davis, H., Bingham, R., Hein, A., Hogg, A., Martín, C., and Thomas, E.: A combined radiostratigraphy- and ice-core- derived age scale for ice at the divide between the Amundsen, Bellingshausen and Weddell seas, West Antarctica, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6677, https://doi.org/10.5194/egusphere-egu25-6677, 2025.

EGU25-7500 | Posters on site | CR2.2

Global High-Resolution Modeling: A New Lens on the Southern Ocean 

Mira Berdahl, Gunter Leguy, Eric J. Steig, William H. Lipscomb, and Bette L. Otto-Bliesner

Modern West Antarctic ice loss is generally driven by warm circumpolar deep water (CDW) reaching ice shelf grounding zones. Understanding what controls CDW delivery remains a challenge, in part because of the multiple scales involved. Most global models are too coarse to capture critical regional processes, while simulations with high-resolution regional models depend on imposed boundary conditions, precluding the possibility of capturing coupled processes across scales.  Here, we analyze a novel multi-member ensemble of global high-resolution (0.1° ocean, 0.25° atmosphere) Community Earth System Model (CESM) simulations over the historical period (1850-2005).   We compare the high-resolution runs to equivalent simulations at ~1 to 2° resolution, as well as to observational products (e.g. ECCO, WOA).  We show that biases in key ocean properties in the Southern Ocean are significantly improved in the high-resolution simulations.  This includes better representation of CDW in the high-resolution runs. We use these comparisons to explore new insights on the atmosphere and ice conditions that promote CDW delivery toward the ice shelves.

How to cite: Berdahl, M., Leguy, G., Steig, E. J., Lipscomb, W. H., and Otto-Bliesner, B. L.: Global High-Resolution Modeling: A New Lens on the Southern Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7500, https://doi.org/10.5194/egusphere-egu25-7500, 2025.

EGU25-7794 | ECS | Posters on site | CR2.2

Short-term variations of spaceborne microwave brightness temperature on the Greenland ice sheet during the 2012 melting season. 

Takumi Suzuki, Rigen Shimada, Misako Kachi, and Tomonori Tanikawa

The accelerated melting of the Greenland ice sheet, driven by recent global warming, has attracted significant attention regarding the long-term variations in its mass balance. While several analyses have utilized snow melting indicators derived from microwave brightness temperatures observed through satellites, there is a lack of studies examining the diurnal behavior of these temperatures during the melting season. The Advanced Microwave Satellite Radiometer 2 (AMSR2) aboard the Global Change Observation Mission – Water (GCOM-W) satellite provides multiple daily observations on the Greenland ice sheet, enabling the investigation of diurnal changes in brightness temperature. This study aims to clarify the short-term relationship between snow melting and spaceborne microwave brightness temperatures during the summer of 2012, a period marked by extensive melting of the Greenland ice sheet. To examine the timing of snowmelt, snow surface temperature data collected by the Automated Weather Station (AWS) at a site on the ice sheet in north-west Greenland were utilized. The time series of snow surface temperatures from July to August 2012 were analyzed, revealing distinct patterns across three periods: Period A (early-July: snow temperature of 0°C only during the day), Period B (mid-July: snow temperature of 0°C throughout the day), and Period C (mid-August: snow temperature below 0°C all day). In the north-west regions, Snow Index (Tb18H − Tb36H: Difference in brightness temperature between 18 GHz-H and 36 GHz-H) values, indicative of snow cover, showed significantly different short-term variations between the periods. During Period A, Snow Index values were positive throughout the day and decreased towards the afternoon. In contrast, during Period B, Snow Index values were negative throughout the day, with no significant diurnal changes observed. During Period C, Snow Index values returned to positive again and, as in the previous period, no significant changes were observed during the day. These results suggest the possibility of monitoring diurnal melting with high temporal resolution through short-term variations in spaceborne microwave brightness temperature. These variations across the Greenland ice sheet, including other frequency channels, will be further discussed during the conference day.

How to cite: Suzuki, T., Shimada, R., Kachi, M., and Tanikawa, T.: Short-term variations of spaceborne microwave brightness temperature on the Greenland ice sheet during the 2012 melting season., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7794, https://doi.org/10.5194/egusphere-egu25-7794, 2025.

EGU25-8670 | ECS | Orals | CR2.2

Unravelling abrupt transitions of Antarctic Ice Sheet dynamics during the mid-Pleistocene transition 

Christian Wirths, Antoine Hermant, Christian Stepanek, Thomas Stocker, and Johannes Sutter

A mechanistic understanding of the main drivers of Quaternary climate variability, especially during the mid-Pleistocene transition (MPT; around 1.2–0.8 million years ago) remains a significant challenge in paleoclimate research. Climate changes during that time include a pronounced shift from 41-kyr to 100-kyr periodicity of glacial cycles as imprinted on sea level reconstructions, and the emergence of much larger ice sheets. While several modeling studies have focused on the interplay between the climate system and northern hemispheric ice sheets during the MPT, the role of Antarctica in driving and responding to climate change at that time remains largely unknown.  

Here, we use the Parallel Ice Sheet Model (PISM) to simulate the transient evolution of the Antarctic Ice Sheet throughout the last 3 million years. PISM is forced by a climate index approach that is based on snapshots of climatic conditions in the past. Climate snapshots are derived from the Community Earth System Models (COSMOS), a general circulation model that simulates atmosphere, ocean, sea ice and land vegetation in dependence of reconstructions of paleogeography, orbital configuration, and greenhouse gas concentrations. Interpolation in times between snapshots is linear and based on a convolution of the EPICA Dome C record and the Lisiecki-Raymo benthic isotope stack.  

Our simulations indicate that between 1.9 Ma and 800 ka BP, several Antarctic drainage basins crossed critical thresholds at different times, for example leading to the formation of a stable marine-based West Antarctic Ice Sheet. We further examine the characteristics of these thresholds and their associated state transitions. Additionally, our findings suggest that these thresholds, and their interplay, amplified eccentricity-driven climate variability both before and during the MPT, providing new insights into the complex interactions between Antarctic ice sheet dynamics and climate during this period. 

How to cite: Wirths, C., Hermant, A., Stepanek, C., Stocker, T., and Sutter, J.: Unravelling abrupt transitions of Antarctic Ice Sheet dynamics during the mid-Pleistocene transition, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8670, https://doi.org/10.5194/egusphere-egu25-8670, 2025.

EGU25-9305 | ECS | Orals | CR2.2

Stability of the Greenland and Antarctic ice sheets coupled by the Atlantic ocean circulation 

Sergio Pérez Montero, Jorge Alvarez-Solas, Alexander Robinson, and Marisa Montoya

Anthropogenic climate change poses a challenge to the stability of current ice sheets. Rising atmospheric temperatures accelerate surface melting in Greenland. Increased ocean temperatures can lead to ice loss at the margins of Antarctica, with positive feedbacks facilitating further ice loss. Both processes impact the Earth System by leading to rising sea level, increasing temperatures through albedo feedbacks, and altering global oceanic circulation. Past records indicate that there is a bipolar interaction between the ice sheets of the Northern and Southern Hemispheres modulated by the Atlantic Meridional Overturning Circulation (AMOC) that could ultimately affect their individual stability. Could the future response of the Greenland and Antarctic ice sheets perturb the AMOC in a manner that changes their own stability landscape? Here we will present the first results of the future evolution of the Greenland and Antarctic ice sheets as simulated with the ice-sheet model Yelmo coupled to a box model representing the oceanic circulation. We will show the coupled effects of the shrinking mass of the ice sheets on the AMOC stability and its feedback on the evolution of the ice sheets themselves.

How to cite: Pérez Montero, S., Alvarez-Solas, J., Robinson, A., and Montoya, M.: Stability of the Greenland and Antarctic ice sheets coupled by the Atlantic ocean circulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9305, https://doi.org/10.5194/egusphere-egu25-9305, 2025.

EGU25-9630 | ECS | Posters on site | CR2.2

Modeling Antarctic Ice Sheet Dynamics in Response to Solar Radiation Management 

Marta Corrà, Antoine Hermant, Daniele Visioni, Paul Brent Goddard, Anthony Jones, Emma Spezia, and Johannes Sutter

The Antarctic Ice Sheet (AIS) could become the largest single contributor to future sea level rise (SLR). However, its response to rising global mean temperature remains highly uncertain, and potential Solar Radiation Modification (SRM) interventions during the 21st century further complicate the projections. Among these interventions, Stratospheric Aerosol Injections (SAI) have been proposed to limit atmospheric warming and potentially moderate or prevent AIS’ impact on SLR. This study examines the dynamic response of Antarctica to such SAI interventions, in the short-term (until the year 2100) and on centennial time scales. We use the Parallel Ice Sheet Model (PISM) forced by the Community Earth System Model 2 (CESM2) to compare the evolution of AIS under SAI scenarios with that under the Shared Socioeconomic Pathway 2-4.5 (SSP2-4.5). Our findings indicate that, on centennial timescales, SAI may be counterproductive in mitigating sea level rise due to the reduced Antarctic surface mass balance compared to the SSP2-4.5 scenario. Ice shelf thinning and grounding line dynamics emerge as dominant factors driving mid- and long-term AIS behavior, where ice dynamics dominate over the effects of constant climate forcing. Variations in the sliding law parameterization further influence simulated outcomes. Unsurprisingly, the results are highly dependent on the individual earth system model employed. To address this, we compare our findings with a suite of the Ice Sheet Model Intercomparison Project for CMIP6 (ISMIP6) scenarios, as well as additional SRM simulations performed using the Hadley Centre Global Environment Model version 2 (HadGEM2-ES).

How to cite: Corrà, M., Hermant, A., Visioni, D., Goddard, P. B., Jones, A., Spezia, E., and Sutter, J.: Modeling Antarctic Ice Sheet Dynamics in Response to Solar Radiation Management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9630, https://doi.org/10.5194/egusphere-egu25-9630, 2025.

EGU25-9731 | ECS | Orals | CR2.2

Simulated ice-ocean-bedrock interactions in Antarctica until year 3000 

Antonio Juarez-Martinez, Jan Swierczek-Jereczek, Javier Blasco, Jorge Alvarez-Solas, Alexander Robinson, and Marisa Montoya

The Antarctic Ice Sheet (AIS) is expected to be one of the dominant contributors to sea level rise in the near future. However, its future sea-level contribution is subject to substantial uncertainties related to modeling of physical processes. One key process is sub-shelf melting, which is particularly important in ice-shelf cavities, where warmer water intrusions could destabilize the corresponding ice shelves. This is of particular interest in the West Antarctic Ice Sheet, where many regions are marine based. Another fundamental process is Glacial Isostatic Adjustment, which is associated with the lithospheric rebound in response to changes in the ice load. Here, we use a 3D ice-sheet-shelf model coupled with a novel isostasy model to analyze the role of interactions between the ice, the ocean and the lithosphere in AIS projections during the next millennium. We combine experiments testing the sensitivity of several parameters concerning basal melting laws and different isostatic adjustment methods, under mean climatic conditions with high and low emissions scenarios. 

 

How to cite: Juarez-Martinez, A., Swierczek-Jereczek, J., Blasco, J., Alvarez-Solas, J., Robinson, A., and Montoya, M.: Simulated ice-ocean-bedrock interactions in Antarctica until year 3000, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9731, https://doi.org/10.5194/egusphere-egu25-9731, 2025.

EGU25-10037 | ECS | Posters on site | CR2.2

Modelling the Northern Hemisphere ice sheet evolution during the last deglaciation and MIS-11 with an ice sheet-ice shelf coupled model 

Wei Liu, Qiuzhen Yin, Philippe Huybrechts, and Heiko Goelzer

Ice sheet models are essential tools for studying ice sheet dynamics in response to the climate evolution during the Quaternary glacial-interglacial cycles. Here, we develop a new version of the Northern Hemisphere ice sheet model (NHISM, Zweck and Huybrechts, 2005) by adding a user-friendly ice shelf module and other new characteristics, such as the configurable horizontal resolution and coupled sea level change. This new ice sheet-ice shelf coupled model is named NHISM1.1. The ice shelf module is based on the shallow shelf approximation, allowing simulation of ice stream advance into the ocean and the transformation between floating and grounded ice. NHISM1.1 is first used to conduct offline equilibrium ice-sheet simulations driven by observed present-day climate. It simulates a reasonable spatial distribution of the Northern Hemisphere ice sheets with a bias of less than 10% in the Greenland Ice Sheet volume compared to observation. We then use NHISM1.1 to perform offline transient ice sheet simulations for two distinct periods in the past, the Last Deglaciation and the entire MIS-11 period. In both cases, NHISM1.1 is driven by climate outputs of transient simulations performed with the LOVECLIM1.3 model. The performance of NHISM1.1 and the influence of various model configurations are evaluated by comparison with proxy reconstructions and other model simulations as well as sensitivity experiments. Our ice sheet simulations show that the NH ice sheets are largely consistent with geological evidence and that the incorporation of an ice shelf module is critical in properly reproducing glacial inception. By combining the analysis of climate simulations from LOVECLIM1.3 and offline ice sheet simulations from NHISM1.1, we propose that insolation plays a dominant role in driving the initial cooling of the Northern Hemisphere and the regrowth of its ice sheets during the MIS-11 glacial inception.

How to cite: Liu, W., Yin, Q., Huybrechts, P., and Goelzer, H.: Modelling the Northern Hemisphere ice sheet evolution during the last deglaciation and MIS-11 with an ice sheet-ice shelf coupled model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10037, https://doi.org/10.5194/egusphere-egu25-10037, 2025.

EGU25-10066 | ECS | Posters on site | CR2.2

Assessing Antarctic Ice Sheet dynamics under temporary overshoot and long-term temperature stabilization scenarios   

Emma Spezia, Marta Corrà, Julien Bodart, Vjeran Višnjević, Fabrice Kenneth Michel Lacroix, Thomas Frölicher, and Johannes Sutter

Current projections of Antarctic Ice Sheet dynamics during the next centuries are subject to large uncertainties both reflecting the ice sheet model setup as well as the climate pathways taken into consideration. Assessing both, we present ice sheet model projections of the Antarctic Ice Sheet’s evolution during the next centuries using PISM. We employ PISM at continental scale forced by Earth system model data tailored to specific global temperature scenarios via an adaptive greenhouse gas emissions approach. The scenarios reflect a range of transient temperature overshoot (during the 21st and 22nd century) and stabilization trajectories until the year 2500 resulting either in 1.5 °C or 3°C warming. We account for various ice sheet sensitivities and initialize PISM with a present-day state obtained by a paleo thermal spin-up and further tuned on present-day conditions. For each climate scenario, a wide range of physical parameterizations is explored, to consider different ice sheet responses. Comparing the results with a historical baseline control simulation, a relative loss of ice volume proportional to temperature rise is observed across all parameters in the various scenarios. Additionally, tipping points can be identified for certain parameterisations, beyond which no significant differences are observed between stabilization and overshoot scenarios indicating an already destabilised West Antarctic Ice Sheet at present. We compare these results with model projections based on a selection of the CMIP6 scenarios to illustrate the range of Antarctic Ice Sheet responses under uncertain future climate trajectories.

How to cite: Spezia, E., Corrà, M., Bodart, J., Višnjević, V., Lacroix, F. K. M., Frölicher, T., and Sutter, J.: Assessing Antarctic Ice Sheet dynamics under temporary overshoot and long-term temperature stabilization scenarios  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10066, https://doi.org/10.5194/egusphere-egu25-10066, 2025.

EGU25-10219 | ECS | Orals | CR2.2

Safety Bands of Thwaites Glacier 

Daniel Moreno-Parada, Violaine Coulon, and Frank Pattyn

Mass loss from the Antarctic Ice Sheet is the main source of uncertainty in projections of future sea-level rise. These uncertainties essentially stem from the fact that some regions, such as Thwaites Glacier, may reach a tipping point, defined as irreversible mass loss on human time scales, with a warming climate. The exact timing of when these tipping points may occur remains difficult to determine, allowing for a large divergence in timing of onset and mass loss in model projections. Previous studies have emphasized the difficulties assessing the most suitable observable and the record length necessary to predict such an abrupt collapse within the Early Warning Indicators (EWI) framework. In particular, Rosier et al. (2021) showed that EWI robustly detect the onset of the marine ice sheet instability in realistic geometries such as Pine Island Glacier. The goal of this work is to determine the physical processes that influence the rate of grounding-line retreat of Thwaites Glacier and to test the capability of EWI to predict the onset of such a collapse. Ultimately, this study aims at mapping potential safety bands of grounding-line positions where the glacier may still recover or alternatively reach a ‘stable’ state. 

How to cite: Moreno-Parada, D., Coulon, V., and Pattyn, F.: Safety Bands of Thwaites Glacier, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10219, https://doi.org/10.5194/egusphere-egu25-10219, 2025.

EGU25-11215 | ECS | Posters on site | CR2.2

Extending our knowledge of Antarctic SMB further back in time 

Damien Maure, Christoph Kittel, Clara Lambin, Quentin Dalaiden, Hugues Goosse, and Xavier Fettweis

The reconstruction of Antarctic surface mass balance (SMB) is essential for understanding ice sheet dynamics and sea level rise, yet existing datasets are limited to the satellite era (1979-present) because little is known about the sea surface conditions (SSCs) before 1979. Using a new SSCs product derived from a particle filtering reconstruction of the southern climate before 1979 to constrain the regional atmospheric model MAR, we expand the known SMB time series up to 1958. The dataset has been evaluated against AWS and SMB measurement campaigns to ensure a good agreement throughout the simulation period, substantially better than when MAR is forced by ERA5 SSCs (HadISST2). We also investigate the influence of the sea ice extent drop on SMB observed between the 70s and the 80s, analogous to the one observed in 2016. This extended dataset offers improved insight into past ice sheet mass changes and highlights the importance of long-term SMB reconstructions for further understanding the role of the Antarctic ice sheet in Earth's climate system.

How to cite: Maure, D., Kittel, C., Lambin, C., Dalaiden, Q., Goosse, H., and Fettweis, X.: Extending our knowledge of Antarctic SMB further back in time, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11215, https://doi.org/10.5194/egusphere-egu25-11215, 2025.

EGU25-11339 | ECS | Posters on site | CR2.2

A Greenland-wide Holocene deglaciation model and building an accompanying 14C database 

Astrid Rosenberg, Gregor Luetzenburg, Ole Bennike, Kristian Kjellerup Kjeldsen, and Nicolaj Krog Larsen

The timing of the Greenland Ice Sheet's retreat from its extent during the Last Glacial Maximum is a key element in constraining the sensitivity of the ice sheet to climate forcing. Although different deglaciation models have been published in previous years (Bennike, 2002; Funder et al., 2011; Sinclair et al., 2016; Leger et al., 2024), these models are limited by the number of samples used or their geographical extent. Therefore, the models have not been able to adequately resolve the deglaciation chronology of the Greenland Ice Sheet.

In this project, we aim to develop a Greenland-wide deglaciation model based on a new compilation of 14C dates, cosmogenic nuclide dates, OSL dates, and geomorphological evidence. The new compilation of 14C samples will be provided as an open-access database: GreenDated.

Within GreenDated, we aim to include all published 14C data from Greenland and the surrounding ocean shelf. All sample entries will as a minimum include information on location, and a categorization of the depositional environment and the sampled material. These steps will ensure accessibility for future users and enable easy extraction of data from the database. We will also recalibrate all the 14C data using the newest calibration curves (Heaton et al., 2020; Reimer et al., 2020) and adjust for differences in old normalization techniques, enabling easy recalibration of data for future users. Lastly, we will conduct a quality assessment based on the protocol used in the Dated (Hughes et al., 2016) and SvalHola (Farnsworth et al., 2020) databases, with the addition of an automated scoring system, seeking to limit bias from the authors.

Ultimately, the deglaciation model and the accompanying GreenDated database will provide a complete and thorough constraint on the Greenland Ice Sheet’s retreat from the Last Glacial Maximum position.

References:
Bennike, O. (2002) ‘Late Quaternary history of Washington Land, North Greenland’, Boreas, 31(3), pp. 260–272. https://doi.org/10.1111/j.1502-3885.2002.tb01072.x.
Farnsworth, W.R. et al. (2020) ‘Holocene glacial history of Svalbard: Status, perspectives and challenges’, Earth-Science Reviews, 208, p. 103249. https://doi.org/10.1016/j.earscirev.2020.103249.
Funder, S. et al. (2011) ‘The Greenland Ice Sheet During the Past 300,000 Years: A Review’, Developments in Quaternary Science, 15, pp. 699–713. https://doi.org/10.1016/B978-0-444-53447-7.00050-7.
Heaton, T.J. et al. (2020) ‘Marine20—The Marine Radiocarbon Age Calibration Curve (0–55,000 cal BP)’, Radiocarbon, 62(4), pp. 779–820. https://doi.org/10.1017/rdc.2020.68.
Hughes, A.L.C. et al. (2016) ‘The last Eurasian ice sheets – a chronological database and time-slice reconstruction, DATED-1’, Boreas, 45(1), pp. 1–45.  https://doi.org/10.1111/bor.12142.
Leger, T.P.M. et al. (2024) ‘A Greenland-wide empirical reconstruction of paleo ice sheet retreat informed by ice extent markers: PaleoGrIS version 1.0’, Climate of the Past, 20(3), pp. 701–755. https://doi.org/10.5194/cp-20-701-2024.
Reimer, P.J. et al. (2020) ‘The IntCal20 Northern Hemisphere Radiocarbon Age Calibration Curve (0–55 cal kBP)’, Radiocarbon, 62(4), pp. 725–757. https://doi.org/10.1017/rdc.2020.41.
 inclair, G. et al. (2016) ‘Diachronous retreat of the Greenland ice sheet during the last deglaciation’, Quaternary Science Reviews, 145, pp. 243–258. https://doi.org/10.1016/j.quascirev.2016.05.040.

How to cite: Rosenberg, A., Luetzenburg, G., Bennike, O., Kjellerup Kjeldsen, K., and Krog Larsen, N.: A Greenland-wide Holocene deglaciation model and building an accompanying 14C database, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11339, https://doi.org/10.5194/egusphere-egu25-11339, 2025.

EGU25-11420 | ECS | Orals | CR2.2

New monthly maps of accumulation over the Greenland Ice Sheet 

Josephine Lindsey-Clark, Aslak Grinsted, and Christine Hvidberg

The Greenland Ice Sheet (GrIS) has become the single largest contributor to present day sea-level rise, with mass loss driven by changes in Surface Mass Balance (SMB). As the largest component of SMB, snow accumulation is critical to monitor as Arctic warming continues at an accelerated rate. Snowfall patterns across GrIS are influenced by a complex interaction of many interdependent climate variables, leading to high inter-annual spatial variability. As a result, regional climate models (RCMs) often fail to adequately capture this variability and carry substantial uncertainties, leading to biased estimations of ice mass loss. Here, we present a novel method to bias-adjust RCM precipitation output with in-situ SMB records from the SUMup dataset (2024 release), including over two million data points from radar, ice-core, snow pit and stake measurements. RCM output data is first decomposed into Empirical Orthogonal Functions (EOFs), reflecting different modes of spatial variability, and Principal Components (PCs), capturing temporal fluctuations correlating to various climate indices. The SUMup in-situ measurements are used to derive a set of coefficients to scale the model mean climatology and each EOF and PC through least-squares optimisation. We provide monthly bias-adjusted accumulation maps for HIRHAM5-ERA5 output between 1960-2023 and CARRA between 1991-2023, highlighting regional biases in the models through time. 

Preliminary mean bias maps for HIRHAM5 show that the model underestimates accumulation in the south and interiors of the ice sheet by 20-80% or 30-90 mm/year, while the west and east margins of the accumulation zone are overestimated by 20-60% or 30-150 mm/year. In the winter and spring, the model tends to underestimate accumulation overall by 50-100 mm/year, while the reverse is true for the summer and autumn, when accumulation is mostly overestimated, reaching up to 200 mm/year in the north west. 

How to cite: Lindsey-Clark, J., Grinsted, A., and Hvidberg, C.: New monthly maps of accumulation over the Greenland Ice Sheet, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11420, https://doi.org/10.5194/egusphere-egu25-11420, 2025.

EGU25-11651 | ECS | Posters on site | CR2.2

Towards understanding the effects of extreme events on Antarctic ice-sheet dynamics  

Lena Nicola, Johanna Beckmann, Felicity McCormack, and Ricarda Winkelmann

Projections of Antarctica's future sea-level contribution are still subject to great uncertainties, especially with respect to changes in surface mass balance and sub-shelf melting. While the climatic forcing used as boundary condition for ice sheet models cover the average trend in mass balance with global warming, extreme events, such as heatwaves, are typically not yet considered. However, a number of record-breaking extreme events have been observed in recent years in Antarctica already and may become more frequent or extreme with ongoing climate change. Here we investigate the effects of heatwaves on ice-sheet dynamics: using a storyline approach for conducting a suite of numerical ice-sheet simulations, we explore the additional Antarctic contribution to future sea-level rise when atmospheric extreme events are considered in projections. We set this into perspective with anomalous freshwater fluxes from ocean-driven melting (and calving) and investigate the potential for abrupt shifts and tipping dynamics, which extreme events may cause or pre-condition.

How to cite: Nicola, L., Beckmann, J., McCormack, F., and Winkelmann, R.: Towards understanding the effects of extreme events on Antarctic ice-sheet dynamics , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11651, https://doi.org/10.5194/egusphere-egu25-11651, 2025.

EGU25-11803 | Posters on site | CR2.2

Bridging the gap between the modern and historical: Extending the mass balance reconstruction of the Greenland Ice Sheet from 1421 to 2024 AD 

Leanne Wake, Aaquib Javed, Emily Hill, Edward Hanna, and Hilmar Gudmundsson

Bridging the knowledge gap between the recent decades and the preceding centuries of Greenland Ice Sheet (GrIS) history is essential for improving projections of its contribution to future sea-level rise. Evidence from relative sea-level reconstructions from salt marshes in southern Greenland suggests that GrIS mass loss began around 1850, well before significant anthropogenic warming—a pattern not yet captured in existing simulations of late Holocene GrIS evolution. Extending reconstructions of GrIS surface mass balance (SMB) as far back as possible, by leveraging newly available climate datasets from ~AD 1400 is critical to understanding its sensitivity to climate forcings during key periods such as the Little Ice Age. 

By addressing the underrepresentation of dynamic components and calculation of pre-20th century mass changes, this project aims to provide critical insights into GrIS-climate interactions and refine predictions of GrIS contributions to global sea-level rise. To achieve this aim, we will first  develop a 1x1-km resolution monthly SMB dataset using ModE-RA, a new palaeoclimate reanalysis product spanning 1421-2024.  This new SMB dataset will be used as input to ice sheet model simulations to assess the  spatial and temporal interplay between climate, SMB and ice dynamics.

Here we will present initial results of (1) GrIS temperature, precipitation and SMB fields for 1421 to 2024 AD and (2) historical simulations using the ice sheet model Úa to reconstruct ice thickness and margin changes outside of the observational period.

How to cite: Wake, L., Javed, A., Hill, E., Hanna, E., and Gudmundsson, H.: Bridging the gap between the modern and historical: Extending the mass balance reconstruction of the Greenland Ice Sheet from 1421 to 2024 AD, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11803, https://doi.org/10.5194/egusphere-egu25-11803, 2025.

EGU25-12628 | ECS | Orals | CR2.2

Hysteresis of the Antarctic ice sheet with a coupled climate-ice-sheet model 

Gaëlle Leloup, Aurélien Quiquet, Didier Roche, Christophe Dumas, and Didier Paillard

Anthropogenic greenhouse gas emissions and resulting global warming raise uncertainties in the future of currently existing ice sheets. The Antarctic ice sheet, which contains the equivalent of 58 meters of potential sea level rise, is expected to have a relatively small role on sea level rise in this century, but is expected to continue to lose mass afterwards and could become a major driver of sea level rise on longer timescales (Van Breedam et al., 2020; Winkelmann et al., 2015).

The Antarctic ice sheet interacts with the solid Earth, the ocean and the atmosphere, resulting in various positive and negative feedbacks, enhancing or limiting ice sheet growth (Fyke et al., 2018). Positive feedback mechanisms, such as the albedo-melt and elevation-temperature feedbacks, enhance the ice sheet's response to an initial change in forcing, potentially resulting in nonlinear changes, and it is thus crucial to model these feedbacks on long timescales, when significant changes of the ice sheet’s topography can occur. Nonlinear changes can lead to a hysteresis behaviour, with widely different equilibrium states for a given CO2 level or temperature anomaly, depending on the initial condition (Pollard and de Conto, 2005; Garbe et al., 2020; Van Breedam et al., 2023).

In this study, we explore the hysteresis of the Antarctic ice sheet from the present-day configuration, using an intermediate complexity climate model, iLOVECLIM, representing the atmosphere, ocean and vegetation, coupled to an ice sheet model, GRISLI. Simulations start from either a pre-industrial ice sheet or an ice-free, isostatically rebounded geometry, and different CO2 levels are applied.

Crucially, the albedo-melt feedback is accounted for in our coupled setting, which strengthens nonlinear behaviour and leads to critical CO2 thresholds for the ice sheet melt or growth. This enhances the ice sheet hysteresis, with widely different equilibrium ice volumes at a given CO2 level, depending on the initial ice sheet geometry. The CO2 thresholds either trigger the complete Antarctic ice sheet loss or near-complete regrowth. The orbital configuration influences these CO2 thresholds : a higher (lower) summer insolation in the Southern Hemisphere decreases (increases) the CO2 threshold for Antarctic deglaciation (glaciation).

These findings highlight the importance of ice sheet-atmosphere interactions, notably the albedo-melt feedback, in projecting future long-term ice sheet behavior. Neglecting these feedbacks could lead to an overestimation of CO2 thresholds for the Antarctic ice sheet destabilization, with implications for future long-term sea level rise under high emission scenarios.

This study has recently been accepted in Geophysical Research Letters.

How to cite: Leloup, G., Quiquet, A., Roche, D., Dumas, C., and Paillard, D.: Hysteresis of the Antarctic ice sheet with a coupled climate-ice-sheet model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12628, https://doi.org/10.5194/egusphere-egu25-12628, 2025.

EGU25-13026 | Orals | CR2.2

Climate state dependence of ice sheet variability 

Georgia Grant

Cenozoic climate has evolved through stepwise quasi-equilibrium states in response to declining CO2 concentration. As a result, terrestrial polar ice sheets developed in Antarctica ~35 million years ago describing relatively large glacial-interglacial changes, prior to an increasing marine-based ice sheet component by ~15 Ma with lower glacial-interglacial variability, before returning to large glacial-interglacial amplitudes in response to the intensification of Northern Hemisphere Ice Sheets (~2.7 Ma). While mean surface temperature scales linearly with the total concentration of carbon in the atmosphere, this is not the case for past variations in global mean sea-level whose amplitudes are climate-state (CO2)-dependent. By examining past climate drivers (atmospheric CO2) and the response of ice volume (sea level), polar ice sheets are seen to demonstrate vastly different sensitivities under changing climate states highlighted by the ‘100-kyr’ problem of non-linear ice sheet change.

In this study, a new independent global ice volume (sea-level) record (X-PlioSeaNZ: 3.3 – 1.7 Ma) is used to evaluate the deep-sea oxygen isotope proxy record (δ18Obenthic).  An empirical, power-law relationship emerges between δ18Obenthic and sea-level in contrast to long-standing linear δ18Obenthic calibrations. This relationship suggests relatively higher deep-ocean temperature contribution to δ18Obenthic signal and correspondingly lower global ice volume estimates under warmer past climates. It also demonstrates the need for variable ice volume-δ18Obenthic calibrations in response to the evolving bipolar ice sheet geographies over the last ~3 million years (Myr). Consequently, as the Earth system adjusts to 2-3°C of global warming over the coming decades and centuries, a lower paleo-ice sheet sensitivity (compared to the Last Glacial Maximum) is expected for ice sheet configurations where marine based ice sheets act as a buffer to terrestrial based ice sheets and brings geologic reconstructions into agreement with current projections for future sea-level rise.

How to cite: Grant, G.: Climate state dependence of ice sheet variability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13026, https://doi.org/10.5194/egusphere-egu25-13026, 2025.

EGU25-13742 | Posters on site | CR2.2

Geomorphological and sedimentological evidence of past Greenland Ice Sheet advance and retreat on the continental shelf offshore of SE Greenland as revealed by ‘Kang-Glac’ cruise SD041  

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

Cruise SD041 of the UK research vessel the RRS Sir David Attenborough to the continental shelf offshore of SE Greenland took place in July-August 2024. The cruise was part of the UK NERC-funded ‘Kang-Glac’ project, a large multi-disciplinary, international, research project jointly led by British Antarctic Survey and Durham University, UK. The cruise collected a range of geological, geophysical, oceanographic and biological data from the continental shelf offshore of Kangerlussuaq Fjord, SE Greenland, and in several adjoining fjords. The aim of the Kang-Glac project is to investigate the response of the Greenland Ice Sheet to ocean warming during the last 11,700 years of the Holocene. During the cruise marine geophysical data in the form of multibeam swath bathymetric imagery of seafloor landforms and sub-bottom profiler data of shallow acoustic stratigraphy were collected, in addition to a suite of sediment cores. Data collection targeted a large cross-shelf bathymetric trough (‘Kang-Trough’) which extended from the mouth of Kangerlussuaq Fiord to the edge of the continental shelf, as well as a series of smaller fjords to the northeast. These marine geophysical data and sediment cores provide a clear record of an extensive Greenland Ice Sheet (GrIS) which expanded and retreated across the shelf via Kang-Trough. Landforms comprise well developed streamlined subglacial bedforms which show convergent GrIS flow into the trough, as well as occasional transverse moraines recording episodic retreat. Sediment cores recovered subglacial tills recording a grounded ice sheet in the cross-shelf trough overlain by a range of deglacial glacimarine facies recording retreat by melting and iceberg calving. Cores from the adjacent trough mouth fan on the continental slope targeted glacigenic debris flows which likely were deposited when the GrIS was grounded at the shelf edge and delivered glacigenic debris onto the slope. Collectively the data provide new insights into past GrIS extent, dynamics, and the nature of associated glacigenic sediment delivery from the LGM through the Holocene in the SE sector of the Greenland continental margin.

How to cite: O Cofaigh, C., Hogan, K., Lloyd, J., Hunt, M., Snowman Andresen, C., Larter, R., and Roberts, D.: Geomorphological and sedimentological evidence of past Greenland Ice Sheet advance and retreat on the continental shelf offshore of SE Greenland as revealed by ‘Kang-Glac’ cruise SD041 , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13742, https://doi.org/10.5194/egusphere-egu25-13742, 2025.

EGU25-14498 | ECS | Posters on site | CR2.2

Revisiting Antarctic surface melting under climate change by the end of the 21st century using a simple surface energy balance approach 

In-Woo Park, Emilia Kyung Jin, Won Sang Lee, and Kang-Kun Lee

Extensive surface melting has been observed during the austral summer, particularly in the Antarctic Peninsula and peripheral regions. A warming climate change is expected to further increase both precipitation and surface melting due to rising air temperatures. The precipitation, including both liquid and solid phases, contributes to maintaining ice mass, whereas surface melting reduces ice thickness and promotes hydrofracturing of ice shelves, resulting in acceleration of ice mass loss. The Surface Energy and Mass balance model of Intermediate Complexity (SEMIC) is a cost-effective and simplified model which emulates surface energy and mass balance processes. However, its application to Antarctica has not yet been fully explored. In this study, we assess the performance of SEMIC, forced with daily and monthly ERA5 reanalysis data, in reproducing current surface mass balance (SMB) and surface melting. Furthermore, we evaluate future projections of SMB and surface melting under the sustainable (SSP1-2.6) and high-warming (SSP5-8.5) climate scenarios from CMIP6, extending to the end of the 21st century. Our results reveal that SEMIC effectively represents current SMB and surface melting when driven by both daily and monthly forcing, although it underestimates the extent of surface melting in internal ice sheet. Projections indicate that total surface melting volume under SSP1-2.6 and SSP5-8.5 scenarios is projected to gradually increase to 170.1 ± 65.1 Gt yr-1 and 892.4 ± 505.2 Gt yr-1, respectively, during 2090-2100. Under the warming scenario, the area experiencing surface melting exceeding collapse threshold (> 725 mm yr-1) increases significantly by the mid-21st century. While total precipitation is projected to increase, this is offset by an increase in surface melting, resulting in minimal net changes in SMB by the end of the 21st century.

How to cite: Park, I.-W., Jin, E. K., Lee, W. S., and Lee, K.-K.: Revisiting Antarctic surface melting under climate change by the end of the 21st century using a simple surface energy balance approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14498, https://doi.org/10.5194/egusphere-egu25-14498, 2025.

EGU25-15073 | Posters on site | CR2.2

Version 3 of the Community Ice Sheet Model 

Gunter Leguy, William Lipscomb, Kate Thayer-Calder, Samar Minallah, Michele Petrini, Heiko Goeltzer, Tim van den Akker, Bill Sacks, Mariana Vertenstein, and Mira Berdahl

Version 3 of the Community Ice Sheet Model (CISM) is scheduled for release later this year along with version 3 of the Community Earth System Model (CESM). CISM is a parallel, open-source ice flow code, written in Fortran and Python, which can be run as a standalone ice sheet or glacier model or as a coupled component of CESM and NorESM. The model supports several Stokes-flow approximations and has participated in many community intercomparison projects, including ISMIP6, CalvingMIP, and GlacierMIP3.

CISM3 will include new physics options for basal sliding, basal hydrology, iceberg calving, and extrapolating sub-ice-shelf temperature and salinity. A new initialization procedure allows the rate of ice mass change to match observations at the beginning of a projection simulation.  Coupled CISM–CESM simulations can include two-way climate coupling with multiple ice sheets, including Antarctica. CISM3 also has an exciting new capability to initialize and simulate mountain glaciers.

To improve user experience, CISM3 will include new Python tools for setting up glacier and ice sheet simulations and analyzing ice-sheet-relevant fields from other CESM components. CISM is now more integrated with CESM than ever before, by leveraging the Common Infrastructure for Modeling the Earth (CIME) case control and testing system for verification and validation. 

This presentation showcases examples and results using CISM3’s new tools and capabilities. 

How to cite: Leguy, G., Lipscomb, W., Thayer-Calder, K., Minallah, S., Petrini, M., Goeltzer, H., van den Akker, T., Sacks, B., Vertenstein, M., and Berdahl, M.: Version 3 of the Community Ice Sheet Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15073, https://doi.org/10.5194/egusphere-egu25-15073, 2025.

EGU25-15269 | Orals | CR2.2

Study on the Instability of Two Large Glaciers in Northeast Greenland in Recent 60 Years 

Lu An, Litao Dai, Xingchen Liu, and Rongxing Li

The Nioghalvfjerdsfjorden glacier (NG) and Zachariae Isstrøm (ZI) are major contributors to the mass balance of northeast Greenland, which drain 12% of the Greenland Ice Sheet. Accurate measurements of these two glaciers are crucial to the estimation of the mass balance in northeast Greenland. They also serve as an important parameter for reflecting climate change and predicting future sea level rise. In the past, early ice velocity data were scarce, primarily due to challenges in difficulties in image orthorectification caused by large distortions and low quality in historical remote sensing imagery. We proposed a systematic process for orthorectification of CORONA KH-4A imagery, which has proven to be both efficient and accurate in velocity mapping at a precision of 25m. By employing a hierarchical network densification approach based on ARGON KH-5 and CORONA KH-4A imagery, we have successfully reconstructed the ice flow velocity fields for NG and ZI from 1963 to 1967. Combining with other ice velocity products, we have obtained the ice velocity of NG and ZI spanning a period nearly 60 years. The results indicate that the average ice flow velocity near the grounding line has increased by 12.4% for NG and a substantial 81.4% for ZI from 1963 to 2020. While ZI is experiencing accelerated mass loss, the NG is still in a relatively stable state under the similar climate condition. The slight fluctuations in ice velocity for NG may be due to the unique topography and the hindering effect of ice rises, suggesting the climate change may have a comparatively less impact on it.

How to cite: An, L., Dai, L., Liu, X., and Li, R.: Study on the Instability of Two Large Glaciers in Northeast Greenland in Recent 60 Years, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15269, https://doi.org/10.5194/egusphere-egu25-15269, 2025.

EGU25-15319 | ECS | Posters on site | CR2.2

Modelling future Antarctic climate and surface mass balance with RACMO2.4p1 (2015-2100) 

Marte G. Hofsteenge, Willem Jan van de Berg, Christiaan T. van Dalum, Kristiina Verro, Maurice van Tiggelen, and Michiel van den Broeke

We present the first results of future Antarctic climate simulations with the polar-adapted Regional Atmospheric Climate Model (RACMO2.4p1). As part of the PolarRES project, two climate storylines are explored, examining the response of the Antarctic surface mass balance (SMB) to two plausible future climates with varying degree of Antarctic sea ice loss and changes to upper atmospheric circulation. For this RACMO2.4p1 is run on a 11 km horizontal grid forced with high emission scenario SSP3-7.0 simulations from CESM2 and MPI-ESM for the period 2015-2100. To evaluate the model performance using climate model data, we compare historical simulations (1985-2015) forced by CESM2 and MPI-ESM to those forced by ERA5. We examine shifts in Antarctic precipitation and SMB between the current and future climate, and relate those changes to changes in atmopsheric circulation, atmospheric moisture budget and presence of sea ice.

How to cite: Hofsteenge, M. G., van de Berg, W. J., van Dalum, C. T., Verro, K., van Tiggelen, M., and van den Broeke, M.: Modelling future Antarctic climate and surface mass balance with RACMO2.4p1 (2015-2100), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15319, https://doi.org/10.5194/egusphere-egu25-15319, 2025.

EGU25-15980 | ECS | Posters on site | CR2.2

Preliminary insights into Miocene palaeoprecipitation and palaeotemperature using speleothem fluid inclusion isotopes from eastern North Greenland 

Lena Friedrich, Gabriella Koltai, Gina E. Moseley, György Czuppon, Attila Demény, Jian Wang, Hai Cheng, Anika Donner, Yuri Dublyansky, and Christoph Spötl

The Miocene epoch was a warm period characterised by elevated atmospheric CO₂ levels compared to the present day. These CO₂ concentrations are similar to those predicted for future climate scenarios, making the Miocene an important period to deepen our understanding of warmer climates. While Greenland ice cores have provided highly valuable data for the late Quaternary, terrestrial palaeoclimate archives extending deeper in time in the Arctic remain sparse, leaving a significant gap in our knowledge of Greenland's climate history.

Speleothems are an excellent archive for obtaining high-resolution terrestrial climate data. During speleothem formation, dripwater can be trapped as fluid inclusions, preserving the isotopic signature of ancient meteoric water. This study focuses on four speleothems from a cave in eastern North Greenland. U-Pb dating indicates that the speleothems were deposited during the middle and late Miocene. We analysed the stable H isotopic composition of primary fluid inclusions to reconstruct the isotopic composition of palaeo-dripwater. Carbon and oxygen isotopes of the speleothem calcite were also measured in order to estimate quantitative temperatures for eastern North Greenland during middle and late Miocene. Our initial results show that during such an elevated CO2 world, mean annual air temperatures were substantially elevated above modern values.

Macroscopically, all speleothems are comprised of translucent and light brown calcite. Microscopically, the dominant fabric is coarsely crystalline columnar calcite. Fluid inclusion petrography shows the presence of both fluid inclusion-rich and inclusion-poor areas in the late Miocene speleothems, while primary fluid inclusions are abundant in the two middle Miocene speleothems. The mean water content obtained from crushing varies from 0.2 µL to 1.0 µL between the speleothems.

How to cite: Friedrich, L., Koltai, G., Moseley, G. E., Czuppon, G., Demény, A., Wang, J., Cheng, H., Donner, A., Dublyansky, Y., and Spötl, C.: Preliminary insights into Miocene palaeoprecipitation and palaeotemperature using speleothem fluid inclusion isotopes from eastern North Greenland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15980, https://doi.org/10.5194/egusphere-egu25-15980, 2025.

EGU25-16025 | Orals | CR2.2

Greenland and Antarctica as Interacting Constitutes in AWI-ESM 

Christian Rodehacke, Lars Ackermann, Paul Gierz, Ahmadreza Masoum, and Gerrit Lohmann

It is highly challenging to include both the Antarctic and Greenland ice sheets in a state-of-the-art earth system model. Our presentation demonstrates our system's design, the essential steps before coupling the entire system, the challenges faced in the coupling process, and the initial findings from our series of simulations for warming scenarios spanning the next few centuries until 2500.

We will highlight the existing limitations in the computed climate conditions that affect the behavior of ice sheets. These motivate our system's design. For instance, ocean temperature biases in the marginal seas around Antarctica inhibit its direct use to determine basal melting of floating ice shelves fringing Antarctica despite extensive tuning efforts. As a result, we have developed a flexible framework deemed necessary to adequately represent the currently observed ice sheet state. The still delicate integration of ice sheets into climate models directs the spin-up procedure of ice sheet models. The procedure's results and its consequences are presented and discussed. In particular, the available iceberg calving mechanism has been demanding in our simulations because we allow for freely waxing or waning ice shelf edges around Antarctica, unprecedented in coupled climate-ice sheet model systems.

Finally, the first results of our fully coupled simulations complete the presentation. These focus on the interaction between the climate system and Antarctica or Greenland and its influence on primary climatic conditions. In our model system, interacting ice sheets shape the climate state, creating feedback loops that affect the ice sheet state itself. This interaction may ultimately counteract the disintegration of ice sheets. Supposed it is a robust result, it implies that standalone ice sheet simulations may overestimate future sea level contributions.

How to cite: Rodehacke, C., Ackermann, L., Gierz, P., Masoum, A., and Lohmann, G.: Greenland and Antarctica as Interacting Constitutes in AWI-ESM, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16025, https://doi.org/10.5194/egusphere-egu25-16025, 2025.

EGU25-16564 | Posters on site | CR2.2

Exploring Antarctic Circulation-Ice Sheet Interactions in UKESM Climate Projections Through 2500 and Beyond 

Sarah Taylor, Andrew Orr, Stephen Cornford, Thomas Bracegirdle, and Robin Smith

Understanding how key regional circulation features respond to future global warming is essential for projections of Antarctic Ice Sheet dynamics, and future global sea level rise. The Southern Annular Mode (SAM) influences the strength and location of the mid-latitude tropospheric westerly jet, which controls the transport of warm air and moisture towards the AIS. The Amundsen Sea Low (ASL), a permanent low-pressure system off the coast Antarctica affects regional wind patterns, precipitation and ocean circulation. These features can also impact the exchange of heat and carbon dioxide between the ocean and atmosphere, impacting sea ice extent and the stability of ice shelves. Under global warming scenarios, changes in these atmospheric features may significantly alter surface mass balance, surface melt, temperature and precipitation patterns over the AIS.

This study uses UK Earth System Model (UKESM) overshoot experiments that explore future emission increase, stabilization, and reduction simulations to investigate the interactions between atmospheric circulation features and the Antarctic cryosphere. These idealised simulations are forced only by CO2 concentrations and currently extend up to 650 years duration, allowing exploration of the response of the AIS to a range of global warming scenarios, and asses potential reversibility under future CO2 reduction.

This research utilises these simulations to identify trends in the SAM, ASL and westerly jets. Initial results show a deepening of the absolute pressure of the ASL, a poleward shift and strengthening of the westerly jet, with trends increasing and reversibility diminishing with higher global warming scenarios. These simulations are then used to identify any relationship between these features and trends in temperature, precipitation and surface melt over regions of the AIS and ice shelves, providing insights into the long-term stability of the AIS under varying climate scenarios.

How to cite: Taylor, S., Orr, A., Cornford, S., Bracegirdle, T., and Smith, R.: Exploring Antarctic Circulation-Ice Sheet Interactions in UKESM Climate Projections Through 2500 and Beyond, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16564, https://doi.org/10.5194/egusphere-egu25-16564, 2025.

EGU25-16952 | ECS | Orals | CR2.2

From short-term uncertainties to long-term certainties in the future evolution of the Antarctic Ice Sheet 

Ann Kristin Klose, Violaine Coulon, Tamsin Edwards, Fiona Turner, Frank Pattyn, and Ricarda Winkelmann

The future evolution of the Antarctic Ice Sheet with progressing warming constitutes one of the, if not the main uncertainty in projections of future sea-level change. As the largest potential source of sea-level rise and one of the key tipping elements in the climate system, robust projections are needed to inform coastal adaptation planning worldwide.

Using historically-calibrated perturbed-parameter ensembles of projections with two ice-sheet models, we assess the response of the Antarctic Ice Sheet and associated uncertainties to a wide range of climate futures extending to the year 2300 and beyond.

We show that the near-term projections of the Antarctic Ice Sheet are strongly influenced by ice-sheet model sensitivities, especially under limited warming, until strong changes in Antarctic climate beyond the end of the century, as projected under unmitigated emissions, clearly dominate the ice-sheet evolution. Irrespective of the wide range of uncertainties explored in our ensembles, large-scale ice loss is triggered in both West and East Antarctica under higher warming scenarios, but can be avoided by reaching net-zero emissions well before 2100. This leads to a multi-meter difference in the committed Antarctic sea-level contribution projected under low and very high emission pathways by the end of the millennium. Our results suggest that the next years and decades are decisive for the multi-centennial fate of the Antarctic Ice Sheet.

How to cite: Klose, A. K., Coulon, V., Edwards, T., Turner, F., Pattyn, F., and Winkelmann, R.: From short-term uncertainties to long-term certainties in the future evolution of the Antarctic Ice Sheet, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16952, https://doi.org/10.5194/egusphere-egu25-16952, 2025.

EGU25-17048 | Posters on site | CR2.2

Stability of interior North Greenland – an assessment from GPS and satellite data 

Christine S. Hvidberg, Aslak Grinsted, Kristian Keller, Helle A. Kjær, Nicholas Rathmann, Mikkel L. Lauritzen, Dorthe Dahl-Jensen, Ruth Mottram, Nicolaj Hansen, Martin Olesen, Sebastian Simonsen, Louise S. Sørensen, Anne M. Solgaard, and Nanna B. Karlsson

The mass loss from the Greenland ice sheet has increased over the last two decades, and is now a major contributor to the global mean sea level rise. While the interior of the Greenland ice sheet has remained relatively stable, the mass loss from the ice sheet margins have spread to the north and since 2007 propagated into interior Greenland. We present here an assessment of the interior stability in North Greenland over the last three decades using GPS data, remote sensing data, and climate model output. We compile GPS survey data from interior ice core sites in North Greenland at GRIP (1992-1996), NorthGRIP (1996-2001), NEEM (2007-2015), and EastGRIP (2015-2022), and compare with surface mass balance estimates, and remote sensing observations to assess changes over the last decades. While the surface elevation has remained relatively stable at the northern ice divide sites, an inferred northward migration of the ice divide in Northwest Greenland observed in 2007-2015 coincided with the onset of thinning along the ice margin in the Baffin Bay area. The surface elevation near the summit of the Greenland ice sheet lowered slightly over the last 30 years, during a period of widespread thinning along the western margin. The observations are discussed in relation to regional changes in surface mass balance and the dynamical response to mass loss at the ice margin.

How to cite: Hvidberg, C. S., Grinsted, A., Keller, K., Kjær, H. A., Rathmann, N., Lauritzen, M. L., Dahl-Jensen, D., Mottram, R., Hansen, N., Olesen, M., Simonsen, S., Sørensen, L. S., Solgaard, A. M., and Karlsson, N. B.: Stability of interior North Greenland – an assessment from GPS and satellite data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17048, https://doi.org/10.5194/egusphere-egu25-17048, 2025.

EGU25-17469 | ECS | Posters on site | CR2.2

Modelling the evolution of the Greenland ice sheet over glacial-interglacial cycles 

Isabel Schwermer, Anne Munck Solgaard, Mikkel Langgaard Lauritzen, Brice Noël, Roman Nuterman, and Christine Schøtt Hvidberg

The Greenland ice sheet (GrIS) formed more than 1 Ma ago and has evolved over many glacial-interglacial cycles. As it still adjusts to past changes, correctly capturing its present-day state is essential to accurately predict its future evolution and contribution to sea level rise. Furthermore, the past offers numerous examples of the GrIS‘ response to warmer climates, possibly analogous to its future fate.

Here, the Parallel Ice Sheet Model (PISM) is utilized to investigate the evolution of the GrIS over past glacial-interglacial cycles. For simulations over such long timescales, the computationally inexpensive PDD scheme is commonly used to calculate surface melt. However, PDD schemes do not capture spatial and temporal differences in surface mass balance sensitivity to temperature and cannot drive glacial-interglacial ice volume changes as they neglect the positive feedback between melt and albedo. To address this, we instead use the Diurnal Energy Balance Model (dEBM-simple) module. It takes into account seasonally and latitudinally varying melt contributions from solar shortwave radiation and changes in albedo in addition to temperature-driven melt to achieve a better representation of orbital timescales.

We calibrate PISM-dEBM-simple with present-day melt rates from the regional climate model RACMO. The calibrated model is then used to investigate the different patterns of growth and retreat of the GrIS over the past glacial-interglacial cycles emerging from using the PDD or the dEBM module in PISM. The enhanced sensitivity of the dEBM to insolation results in an earlier and greater mass loss at the onset of the Holocene, primarily from low-elevation regions and ice shelves.

How to cite: Schwermer, I., Munck Solgaard, A., Langgaard Lauritzen, M., Noël, B., Nuterman, R., and Schøtt Hvidberg, C.: Modelling the evolution of the Greenland ice sheet over glacial-interglacial cycles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17469, https://doi.org/10.5194/egusphere-egu25-17469, 2025.

EGU25-17480 | ECS | Posters on site | CR2.2

Does the AMOC strength matter for the Antarctic ice sheet retreat during the penultimate deglaciation?  

Maxence Menthon, Pepijn Bakker, Aurélien Quiquet, and Didier Roche

The Antarctic Ice Sheet has contributed 0 to 7.7m to the global mean sea level during the Last Interglacial, according to recent publications (Barnett et al., 2023; Dyer et al., 2021; Dumitru et al., 2023; Shackleton et al., 2020). This large uncertainty suggests that the Antarctic ice sheet could have been similar to present-day geometry, but it could also have had a major retreat such as the collapse of the West Antarctic Ice Sheet and more. For example, Clark et al. 2020 simulate the West Antarctic Ice Sheet collapse in their modeling work. They suggest that a longer period of reduced Atlantic Meridional Overturning Circulation (AMOC) during the penultimate deglaciation compared to the last deglaciation could have led to greater subsurface warming and subsequent larger Antarctic Ice Sheet retreat. 

Here we study the response of the Antarctic ice sheet during the penultimate deglaciation ( 138–128 ka) to different evolutions of the AMOC. We use the ice sheet model GRISLI (Quiquet et al. 2018), including the recently implemented sub-shelf melt module PICO (Reese et al. 2018). The climate forcings, including Northern Hemisphere ice sheets evolution, are obtained from fully coupled Earth System Model simulations using the intermediate complexity model iLOVECLIM (Roche et al. 2014). We run 2 sets of ice sheet simulations. In the first set the Northern Hemisphere ice sheets are fully coupled and therefore provide freshwater fluxes directly to the oceans according to ice sheets melt (Quiquet and Roche 2024). In the second set the freshwater fluxes given in the North Atlantic Ocean are idealized. With the second set, we also test the impact of the timing and duration of the freshwater flux on the ice sheet retreat. We hypothesize that both the duration and timing of reduced AMOC can significantly affect the sensitivity of the Antarctic Ice Sheet. A larger subsurface warming in the Southern Ocean can be triggered by longer AMOC reduction, and the resilience of the ice sheet to this warming depends on its geometry during the deglaciation.   

How to cite: Menthon, M., Bakker, P., Quiquet, A., and Roche, D.: Does the AMOC strength matter for the Antarctic ice sheet retreat during the penultimate deglaciation? , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17480, https://doi.org/10.5194/egusphere-egu25-17480, 2025.

EGU25-19292 | ECS | Posters on site | CR2.2

Mapping the stability of the Greenland Ice Sheet 

Lucía Gutiérrez-González, Jorge Álvarez-Solas, Marisa Montoya, and Alexander Robinson

In the coming century, the Greenland Ice Sheet (GrIS) is expected to be one of the main contributors to global sea-level rise. In addition, it is thought to be a tipping element due to the existence of positive feedbacks governing its mass balance. Previous studies have explored its stability across a range of temperatures, from present-day conditions to a global warming of 4°C, showing a threshold behavior in its response. However, it is known this threshold has already been exceeded in the past. During the Holocene Thermal Maximum, when Greenland temperatures were 2–4°C warmer than today, the ice sheet retreated beyond its present-day margin but did not fully disappear. Ice losses depend on the level of warming, but also on the rate of forcing and how long the forcing remains above the threshold.  Therefore, we propose studying the stability of the ice sheet over a broader temperature range: from the Last Glacial Maximum to a warming of +4°C,  and examining its current state within the bifurcation diagram. For this purpose, we use the ice-sheet model Yelmo coupled with the regional moisture-energy balance model REMBO and a linear parameterization of the oceanic basal melting.

How to cite: Gutiérrez-González, L., Álvarez-Solas, J., Montoya, M., and Robinson, A.: Mapping the stability of the Greenland Ice Sheet, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19292, https://doi.org/10.5194/egusphere-egu25-19292, 2025.

EGU25-19646 | Orals | CR2.2

Early Results from KANG-GLAC: A Project to Understand Holocene Ice Sheet-Ocean Interaction and Marine Productivity in SE Greenland 

Kelly Hogan, O Cofaigh Colm, Povl Abrahamsen, John Howe, Mark Inall, Jeremy Lloyd, Clara Manno, Christian März, David Roberts, Geraint Tarling, Louise Sime, Jochen Voss, Lev Tarasov, and Camilla Andresen and the SD041 Shipboard Scientific Party

So far, melting of the Greenland Ice Sheet (GrIS) has been the biggest contributor from the Earth’s cryosphere to global sea-level rise. Major uncertainties remain about how oceanic heat is transported across the shelf and through the fjords to the faces of marine-terminating glaciers, and how this affects rates of ice melt and calving. In turn, the increasing supply of meltwater and nutrients to the ocean around Greenland is impacting marine ecosystems as primary productivity rises,  subsequently increasing the potential for  carbon to be buried as “blue carbon” in Greenland’s fjords as warming continues. In July-August 2024, the UK-funded KANG-GLAC project completed a 40-day multidisciplinary research cruise to SE Greenland where the 40-strong scientific party made a suite of integrated geological, ocean and biological observations. The main aims of the project are two-fold. First, it aims to better understand how marine-terminating glaciers respond to oceanic heat on longer timescales (decades to centuries) by reconstructing glacier and ice-sheet behaviour during the Holocene and in particular during the climatic warm period of the Holocene Thermal Maximum. Second, the project will quantify nutrient cycling in the water column and uppermost seafloor sediments in order to improve our knowledge of  marine ecosystem response to meltwater supply from the GrIS.  The cruise on the UK’s premier polar research vessel, the RRS Sir David Attenborough, is the start of a 3.5 year project. Here, we will present an overview of our field observations in this past-to-future project and outline the plans for future data-driven modelling of the Greenland Ice Sheet.

How to cite: Hogan, K., Colm, O. C., Abrahamsen, P., Howe, J., Inall, M., Lloyd, J., Manno, C., März, C., Roberts, D., Tarling, G., Sime, L., Voss, J., Tarasov, L., and Andresen, C. and the SD041 Shipboard Scientific Party: Early Results from KANG-GLAC: A Project to Understand Holocene Ice Sheet-Ocean Interaction and Marine Productivity in SE Greenland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19646, https://doi.org/10.5194/egusphere-egu25-19646, 2025.

EGU25-19795 | ECS | Posters on site | CR2.2

Investigating Osmium Isotopes and Sedimentological Records for the end of the Saalian Glacial from Northwest Baffin Bay 

Sirui Huang, David Selby, Jeremy Lloyd, and Paul Knutz

Understanding the dynamic response of the Greenland Ice Sheet (GrIS) during past climate warmings is essential for predicting its behaviour as global warming accelerates. However, detailed reconstructions of GrIS growth and retreat are limited due to lack of long high-resolution sedimentary records in proximity to its major glacial outlets. Here, new osmium isotope data are presented, from IODP Expedition 400 Hole U1604B, obtained from the lower slope of the Melville Bugt Trough Mouth Fan on the northwest Greenland margin. The osmium isotope analyses are integrated with shipboard sedimentary proxies to trace sediment sources and reconstruct glacial meltwater flux. Preliminary results from the studied interval show sediment proxy variations suggesting significant changes in sediment sources and depositional conditions. Between ~29 and 24 m CSF-A 187Os/188Os are radiogenic (~2.3 – 2.5). In contrast, immediately above this section between ~24 and 22 m CSF-A depth 187Os/188Os are distinctly less radiogenic (~1.3). The latter depth interval is also characterized by a peak in Ca/K ratios, decreased magnetic susceptibility and natural gamma radiation. The current preliminary age-model for Hole 1604B suggests that the studied core interval could represent the end of the Saalian Glacial. As such, we hypothesize the change in the sediment proxies is interpreted to record enhanced glacial meltwater and sediment delivery, potentially following ice sheet break-up at the end of the Saalian glacial and transition into the Eemian interglacial. Our multi-proxy findings provide new insight into the relationship between GrIS, Innuitian/Laurentide Ice Sheets, and regional sedimentation patterns during a significant glacial to interglacial transition, with important implications for understanding of GrIS response to abrupt climate warming.

How to cite: Huang, S., Selby, D., Lloyd, J., and Knutz, P.: Investigating Osmium Isotopes and Sedimentological Records for the end of the Saalian Glacial from Northwest Baffin Bay, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19795, https://doi.org/10.5194/egusphere-egu25-19795, 2025.

EGU25-20400 | Posters on site | CR2.2

Coupling the polar ice sheets to the Norwegian Earth System Model: advances and challenges 

Michele Petrini, Mariana Vertenstein, Heiko Goelzer, William H. Lipscomb, Gunter R. Leguy, William J. Sacks, Katherine Thayer-Calder, David M. Chandler, and Petra M. Langebroek

The polar ice sheets are melting faster due to climate change, with the contribution of the Greenland and Antarctic ice sheets being the largest uncertainty in projecting future sea level rise. Understanding this is crucial for assessing impacts on the environment and ecosystems. Most of the existing modelling studies focus on ice sheet response to atmospheric and oceanic forcing. However, the ice sheets closely interact with and influence the Earth’s climate. With the goal of better representing ice sheet and climate processes and feedbacks, we aim to integrate Greenland and Antarctic dynamic ice sheet components into the Norwegian Earth System Model (NorESM). NorESM is a global, CMIP-type coupled model for the physical climate system and biogeochemical processes over land, ocean, sea ice and atmosphere. In its latest release, NorESM features interactive coupling with a dynamic Greenland Ice Sheet (GrIS) component, although this coupling does not explicitly include ocean forcing at the marine-terminating margins of the ice sheet. In this presentation, we will show preliminary results of NorESM simulations featuring (1) a new interactive coupling with the Community Ice Sheet Model (CISM) over both the Antarctic and Greenland domains, and (2) a new ocean and ice sheet coupling allowing us to force the ice sheets with horizontally and vertically resolved  NorESM ocean properties. We will discuss work in progress, highlighting recent advances and most pressing challenges of our coupling approach.

How to cite: Petrini, M., Vertenstein, M., Goelzer, H., Lipscomb, W. H., Leguy, G. R., Sacks, W. J., Thayer-Calder, K., Chandler, D. M., and Langebroek, P. M.: Coupling the polar ice sheets to the Norwegian Earth System Model: advances and challenges, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20400, https://doi.org/10.5194/egusphere-egu25-20400, 2025.

EGU25-20846 | ECS | Orals | CR2.2

The role of Greenland ice sheet – climate interactions from 1000-year coupled simulations with MAR-GISM 

Chloë Paice, Xavier Fettweis, and Philippe Huybrechts

As the second largest ice body on Earth, comprising an ice volume of 7.4 m sea level equivalent, the Greenland ice sheet is one of the main contributors to global sea level rise. Though observational and modelling efforts have increased substantially in recent years, major uncertainties remain regarding the ice sheet – climate interactions and feedback mechanisms that drive the ice sheet’s long-term mass loss. To improve sea level projections and the representation of such interactions in model simulations, efforts are currently emerging to couple ice sheet and regional climate models. However, so far, only a few coupled ice sheet – regional climate model simulations have been performed, and these do not extend beyond the centennial timescale. They therefore provide limited insights into the evolution and critical thresholds of the ice sheet – climate system over longer timescales.

As such, to obtain a better understanding of the ice sheet – climate interactions and potential feedback mechanisms over Greenland, we coupled our Greenland Ice Sheet Model (GISM) with a high-resolution regional climate model, the Modèle Atmosphérique Régional (MAR), and performed millennial-length simulations. The global climate model forcing for MAR during these simulations consisted of the IPSL-CM6A-LR model output under the SSP5-8.5 scenario, which was available until 2300. After this date, the climate was held constant, and we prolonged our coupled simulations until the year 3000.

Specifically, we performed three coupled simulations for the period 1990-3000 with differing coupling complexity: full two-way coupling, one-way coupling and zero-way coupling. In the two-way coupled set-up, the ice sheet topography and surface mass balance were communicated yearly between both models, such that ice sheet – climate interactions were fully captured. In the one-way coupled set-up only the surface mass balance – elevation feedback was considered, through interpolation of the yearly SMB onto the changing ice sheet topography. And lastly, in the zero-way coupled set-up the ice sheet – climate interactions were entirely omitted.

The results show that the ice sheet evolution is determined by positive as well as negative feedback mechanisms, that act over different timescales. The main observed negative feedback in our simulations is related to changing wind speeds at the ice sheet margin, due to which the integrated ice mass loss remains fairly similar for all simulations up to 2300, regardless of the differently evolving ice sheet geometries. Beyond this time however, positive feedback mechanisms related to decreasing surface elevation and changing precipitation patterns dominate the ice sheet – climate system and strongly accelerate the integrated ice mass loss. Hence, over longer timescales and for a realistic representation of the evolving ice sheet geometry, it is indispensable to account for ice sheet – climate interactions as was done in our two-way coupled ice sheet – regional climate model set-up.

How to cite: Paice, C., Fettweis, X., and Huybrechts, P.: The role of Greenland ice sheet – climate interactions from 1000-year coupled simulations with MAR-GISM, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20846, https://doi.org/10.5194/egusphere-egu25-20846, 2025.

EGU25-21018 | ECS | Orals | CR2.2

Mass Recharge of the Greenland Ice Sheet driven by an IntenseAtmospheric River 

Hannah Bailey and Alun Hubbard

Atmospheric rivers are transient channels of intense water vapor that account for up to 90% of the poleward moisture transport from mid-latitudes. Though short-lived, these events can deliver extreme amounts of heat and rainfall that have been widely reported to accelerate ablation and ice mass loss across the Arctic. However, the impact of atmospheric river fueled snowfall has received less attention, partly due to the limited availability of empirical evidence and direct observations. Here, we explore the potential of atmospheric rivers to deliver intense snowfall to the Greenland ice sheet and thereby replenish its health through enhanced mass accumulation. Specifically, we use new firn-core isotopic analyses and glacio-meteorological datasets from Southeast Greenland to examine the origin and impact of atmospheric rivers on regional mass balance. To this end, we sampled firn core stratigraphy from the upper accumulation area of Southeast Greenland and related it to meteorological observations, to demonstrate that an intense atmospheric river in mid-March 2022 delivered up to 11.6 gigatons per day of extreme snowfall to this region of the ice sheet. 
We show that this immense snowfall not only recharged the snowpack and offset Greenland ice sheet net mass loss by 8% in 2022, but also raised local albedo thereby delaying the onset of summer bare-ice melt by 11 days, despite warmer than average spring temperatures. Since 2010, synoptic analysis of ERA5 data reveals that snow accumulation across Southeast Greenland increased by 20 mm water equivalent per year, driven by enhanced Atlantic cyclonicity. Depending on their seasonal timing, our study demonstrates that the impact of atmospheric rivers on the mass balance of the Greenland ice sheet is not exclusively negative. Moreover, their capacity to contribute consequential ice mass recharge may become increasingly significant under ongoing Arctic amplification and predicted poleward intrusion of mid-latitude moisture.

How to cite: Bailey, H. and Hubbard, A.: Mass Recharge of the Greenland Ice Sheet driven by an IntenseAtmospheric River, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21018, https://doi.org/10.5194/egusphere-egu25-21018, 2025.

A major obstacle in both paleo and future simulations of the Antarctic Ice Sheet is that most studies do not include interactive ice sheets. Although this is a current area of development, most studies use stand alone climate models to force separate ice sheet models to study the potential impacts of climate changes on ice sheets; however this method ignores consequent impacts of the ice sheets on the ocean-atmosphere system, leading to simulations that may under or over estimate retreat in a warmer climate. The few model simulations that do include ice sheet-climate feedbacks disagree on the overall sign of the these feedbacks.
Here we are developing a new coupling between an established ice sheet (PSU-ISM) and climate model (HadCM3) that has been used extensively for paleoclimate applications. These models are suitable for performing multiple simulations over thousands of years. The ice sheet model output will be used to update the ice sheet in the climate model. The climate model orography and land sea mask will be modified to match that in the ice sheet model and ice sheet discharge will be added as a freshwater flux, modelled via change in salinity around the Southern Ocean. The models have been coupled offline and we are next automating this process so that simulations can be repeated over shorter timescales. This will allow the model to develop feedbacks more quickly rather than being limited to the length of the run. The model has been developed using pre-industrial idealised simulations. The main focus of the work is on reproducing the AIS response and sea level rise during the middle Miocene warm interval that matches proxy records more closely without having to add unrealistic CO2 forcing.

How to cite: Byrne, L.: Development of a new coupled ice sheet-climate model for simulations of the Antarctic Ice Sheet under a warm climate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21116, https://doi.org/10.5194/egusphere-egu25-21116, 2025.

NP4 – Time Series and Big Data Methods

EGU25-453 | ECS | Orals | SM2.2

Enhancing seismic monitoring with Virtual Seismic Arrays: Application of a deep learning framework 

Jana Klinge, Sven Schippkus, and Céline Hadziioannou

Seismic arrays are essential for collecting and analyzing seismic data, significantly enhancing our understanding of geophysical processes such as the localization of seismic sources. We introduce the concept of Virtual Seismic Arrays, where the array recordings are predicted from a single reference station, removing the need for continuous deployment of all array stations. This work builds on the research by Klinge et al. (2025), which introduced a Deep Learning approach using encoder-decoder networks to learn and predict transfer properties between two seismic stations. By training the algorithm on data of the Gräfenberg array in the secondary microseism frequency band, we develop models that effectively capture the transfer characteristics between a chosen reference station and each of the other stations within the array. To evaluate how well the models represent the underlying wave propagation, we use beamforming and apply it to both the original data from all stations and the corresponding predictions generated by the models. We assess two scenarios: one where the dominant backazimuths and slownesses are consistent with the training dataset, and another where the models are applied to data from different conditions. Our results show strong agreement between the predicted and original beamforming results, demonstrating the potential of Virtual Seismic Arrays for future application.

How to cite: Klinge, J., Schippkus, S., and Hadziioannou, C.: Enhancing seismic monitoring with Virtual Seismic Arrays: Application of a deep learning framework, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-453, https://doi.org/10.5194/egusphere-egu25-453, 2025.

EGU25-739 | ECS | Posters on site | SM2.2

Optimizing neural network architectures and using clustering to detect seismic events in noisy ocean bottom seismometer data 

Alicia Ximena Cortés Barajas, Marco Calò, Erik Molino Minero Re, and Francesca Di Luccio

Detecting seismic events is essential for monitoring tectonic and volcanic activity, especially in marine environments where noise makes analysis particularly challenging. This study introduces a method that combines Evolutionary Neural Architecture Search (ENAS) with the third generation of the Non-dominated Sorting Genetic Algorithm (NSGA-III) to design and optimize neural networks for seismic event detection using Ocean Bottom Seismometers (OBS) data.

In this work we developed a methodology to analyze heavily noisy data recorded by the TYDE OBS experiment in the southern Tyrrhenian Sea, Italy. In 2000, 14 seismic stations were deployed on the seafloor and around the Aeolian Islands recording data for about 6 months. Stations consisted of wide-band Ocean Bottom Seismometers (OBS) and Hydrophones (OBH).

The preprocessing pipeline includes feature extraction with Discrete Wavelet Transform (DWT) and dimensionality reduction using Principal Component Analysis (PCA), which reduces over 6000 coefficients to just 55 while preserving 95% of the variance. Applied to 90-second overlapping windows, this approach has achieved strong results, with F1 scores exceeding 90% in balanced noisy datasets.

Building on these results, this study explores unsupervised clustering to group similar seismic events and identify possible false positives through anomaly detection. By using adaptive clustering methods that determine the optimal number of clusters based on the data, this approach aims to enhance reliability while providing additional insights into the detected seismic events.

This work highlights the potential of automated tools to complement traditional seismic monitoring methods, balancing accuracy and model complexity while improving efficiency in noise-heavy environments.

How to cite: Cortés Barajas, A. X., Calò, M., Molino Minero Re, E., and Di Luccio, F.: Optimizing neural network architectures and using clustering to detect seismic events in noisy ocean bottom seismometer data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-739, https://doi.org/10.5194/egusphere-egu25-739, 2025.

EGU25-2833 | ECS | Orals | SM2.2

Unsupervised exploration of seismic activity at Mount Fuji, Japan 

Adèle Doucet, Léonard Seydoux, Nobuaki Fuji, Yosuke Aoki, and Jean-Philippe Métaxian

Mount Fuji volcano, located 100~km away from Tokyo, directly threatens over 30~million people. It last erupted in 1707, and has remained dormant since then. Seismicity --and particularly Low-Frequency Earthquakes (LFE)-- is to now the primary indicator of processes occurring beneath the volcano and is usually linked to fluid movement. Yet, these signals are usually manually picked and classified as such, without the ability to formally define them for automatic detection systems. 

Our goal is to develop an automatic method to detect and classify LFEs, among other seismic events at Mount Fuji using the continuous seismic records from 2008 at 11 stations. First, we use the CovSeisNet software to detect events by analyzing the wavefield coherence, derived from the network covariance matrix width. Over one year of continuous data, the wavefield coherence shows distinct patterns that correspond to various event types, including LFEs and tectonic earthquakes. To enable interpretation, we apply a manifold learning algorithm (UMAP) to reduce the dimension of the coherence patterns into two dimensions to ease the interpretation. We name this low-dimensional representation a "coherence atlas" where each point represents a time window of seismic data, grouped by similarity. This automatic approach enables not only the detection but also the classification of seismic events, as compared with the Japan Meteorological Agency catalog. Moreover, the atlas helps identify previously unrecorded events and facilitates the definition of new event classes. By autonomously mapping and classifying seismic activity beneath Mount Fuji, this method offers unprecedented insights into its activity and allows us to detect new events that had been hidden in the manually prepared catalog.

How to cite: Doucet, A., Seydoux, L., Fuji, N., Aoki, Y., and Métaxian, J.-P.: Unsupervised exploration of seismic activity at Mount Fuji, Japan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2833, https://doi.org/10.5194/egusphere-egu25-2833, 2025.

EGU25-2836 | ECS | Orals | SM2.2

PEGSGraph: A Graph Neural Network for Fast Earthquake Characterization Based on Prompt ElastoGravity Signals 

Céline Hourcade, Kévin Juhel, and Quentin Bletery

State-of-the-art earthquake early warning systems use the early records of seismic waves to estimate the magnitude and location of the seismic source before the shaking and the tsunami strike. Because of the inherent properties of early seismic records, those systems systematically underestimate the magnitude of large events, which results in catastrophic underestimation of the subsequent tsunamis. Prompt elastogravity signals (PEGS) are low-amplitude, light-speed signals emitted by earthquakes, which are highly sensitive to both their magnitude and focal mechanism. Detected before traditional seismic waves, PEGS have the potential to produce unsaturated magnitude estimates faster than state-of-the-art systems. Accurate instantaneous tracking of large earthquake magnitude using PEGS has been proven possible through the use of a Convolutional Neural Network (CNN). However, the CNN architecture is sub-optimal as it does not allow to capture the geometry of the problem. To address this limitation, we design PEGSGraph, a novel deep learning model relying on a Graph Neural Network (GNN) architecture.
PEGSGraph accurately estimates the magnitude of synthetic earthquakes down to Mw~7.6-7.7 and determines their focal mechanisms (thrust, strike-slip or normal faulting) within 70 seconds of the event's onset, offering crucial information for predicting potential tsunami wave amplitudes. Our comparative analysis on Alaska and Western Canada data shows that PEGSGraph outperforms PEGSNet, providing more reliable rapid magnitude estimates and enhancing tsunami warning reliability.

How to cite: Hourcade, C., Juhel, K., and Bletery, Q.: PEGSGraph: A Graph Neural Network for Fast Earthquake Characterization Based on Prompt ElastoGravity Signals, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2836, https://doi.org/10.5194/egusphere-egu25-2836, 2025.

The mechanics of slow frictional creep in landslides remains debated and only a few detailed seismic studies have been conducted in landslide-prone areas. To illuminate basal slip processes for a slow moving landslide, we deployed a dense 80 node seismic array at Oak Ridge Earthflow in California’s Diablo Range for one to two months during the rainy seasons of 2023 and 2024, both winters where decimeters of landslide displacement occurred at Oak Ridge. Simultaneously, GNSS receivers, strain meters, and piezometers were deployed at the same site. During our deployments, various types of very small signals were recorded by the seismometers. These events were local, detected only by nearby stations sited within about 100 m of each other. The cause of these events remains unclear, whether due to shear slip at the base of the earthflow or other sources, such as water movement or animal activity. To investigate the cause of these signals, and evaluate the role of stick-slip motion and shear localization, we automatically detected the events and analyzed their spatiotemporal distribution. We used quakephase (Shi et al., 2024) to identify the phases of the very small signals. The primary challenge with automatic picking in our dataset is the long processing time due to high sampling rates. To address this issue, we applied array signal processing, covseisnet (Seydoux et al., 2016), to extract signal candidates based on the coherence of dominant frequencies across the seismic array, followed by automatic picking. This approach successfully and efficiently identified specific signals we believe are associated with earthflow motion. These signals are not continuously observed but concentrate within specific time periods. We focused on events in these time periods, utilizing scattering networks and matched-filter techniques for more detailed classification. By combining our results with other temporal data, such as pore fluid pressure, precipitation, temperature, and displacement, we will discuss the causes of these signals to better understand the mechanism of the earthflow motion.

How to cite: Iwasaki, Y., Schwartz, S., and Finnegan, N.: Classification of Small Seismic Signals Associated with the Oak Ridge Earthflow in California Using a Combination of Machine Learning and Array Signal Processing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5384, https://doi.org/10.5194/egusphere-egu25-5384, 2025.

EGU25-5429 | ECS | Posters on site | SM2.2

Deep-learning-based dual model with an iterative prediction process for the improvement of missing well-log predictions  

Jaesung Park, Jina Jeong, and Mbarki Sinda

Traditional well-log analysis often involves incomplete datasets, which reduces the accuracy of petrophysical assessments. This study thus introduces an innovative dual-model approach that integrates a conditional variational autoencoder (CVAE) with a long short-term memory (LSTM) to predict missing shear-slowness (DTS) data and other well-log data. Utilizing well-logs and the corresponding lithological sequence from the Volve oil field in the North Sea, the proposed model demonstrates excellent prediction capabilities when facing multiple types of missing well-logs. Our findings reveal that the CVAE-LSTM model not only enhances DTS prediction accuracy but also adapts to the inherent variability of geological formations. It outperforms traditional autoencoder and standalone LSTM models across a range of metrics, including correlation coefficients, the root mean squared error, and Kolmogorov–Smirnov statistics, validating the predictive accuracy of the proposed model and the alignment of the statistical distributions for predicted and actual logs. The robustness of the proposed model is further highlighted by its ability to maintain its high performance despite the absence of key well-log data such as compressional slowness and the neutron porosity index. This study demonstrates the effectiveness of advanced machine-learning techniques in overcoming the limitations associated with incomplete well-log datasets.

How to cite: Park, J., Jeong, J., and Sinda, M.: Deep-learning-based dual model with an iterative prediction process for the improvement of missing well-log predictions , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5429, https://doi.org/10.5194/egusphere-egu25-5429, 2025.

EGU25-6412 | ECS | Posters on site | SM2.2

Enhancing seismicity detection and characterization in the Val d’Agri region: insights into tectonic and induced processes using Deep Learning techniques 

Elisa Caredda, Andrea Morelli, Maddalena Errico, Giampaolo Zerbinato, Marius Paul Isken, and Simone Cesca

Monitoring microseismicity is fundamental to advancing our understanding of fault mechanics under natural and anthropogenic influences. Recent advancements in seismological methodologies, particularly those employing deep learning techniques, have significantly improved the detection of weak earthquakes while preserving high levels of precision and reliability.

This study aims to enhance the detection and characterization of seismicity in the Val d’Agri region (Southern Italy) by implementing advanced deep learning-based methodologies, focusing on understanding the tectonic and anthropogenic influences driving seismic activity. The Val d’Agri region is a tectonically active area of considerable scientific and industrial relevance, hosting Europe’s largest onshore oil reservoir and an artificial lake. By employing state-of-the-art deep learning and full waveform earthquake detection methods we identified and located seismic events over a three-year period, achieving a twofold increase in detected events compared to the manually revised bulletin, with a recall rate of ~95%.

Spatial and temporal analyses, based on a density-based clustering approach, revealed distinct seismic clusters. The seismicity is mostly concentrated along the Monti della Maddalena fault system in the southwestern region, characterized by shallow earthquakes (5–7 km depth), while the northeastern and northwestern areas exhibit sparser and deeper activity (15–20 km depth). High-resolution event localization illuminated fault geometries and spatial distributions with high detail. Additionally, our dataset highlights a temporal correlation between seismicity rates and the filling and emptying phases of the Pertusillo artificial reservoir.

Our findings underscore the utility of automated workflows in improving seismic monitoring and fault characterization, providing critical insights into tectonic processes and reservoir-induced seismicity.

How to cite: Caredda, E., Morelli, A., Errico, M., Zerbinato, G., Isken, M. P., and Cesca, S.: Enhancing seismicity detection and characterization in the Val d’Agri region: insights into tectonic and induced processes using Deep Learning techniques, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6412, https://doi.org/10.5194/egusphere-egu25-6412, 2025.

EGU25-6730 | Posters on site | SM2.2

Readapting PhaseNet to Laboratory Earthquakes: AEsNet, a Robust Acoustic Emission Picker Illuminating Seismic Signatures of Different Fault Gouge Materials 

Marco Maria Scuderi, Giulio Poggiali, Federico Pignalberi, and Giacomo Mastella

Laboratory acoustic emissions (AEs), resembling small-scale earthquakes, provide vital insights into frictional instability mechanics. Recent advancements in acoustic monitoring technology allow for the rapid collection of thousands of AE waveforms within minutes, highlighting the critical need for efficient detection and analysis methods. This study presents a deep learning model designed to automatically detect AEs in laboratory shear experiments.

Our dataset comprises approximately 30,000 manually identified AE waveforms obtained under varying experimental boundary conditions using two fault gouge materials: Min-U-Sil quartz gouge and glass beads. We modified the PhaseNet model, originally designed for detecting seismic phases in natural earthquakes, by optimizing its architecture and training process to develop AEsNet—an advanced AE detection model that consistently outperforms existing picking methods for Min-U-Sil quartz gouge and glass beads.

To assess the model's generalizability across different boundary conditions and materials, we employed transfer learning, examining performance relative to training dataset size and material diversity. Results indicate that while model performance remains consistent across varying boundary conditions, it is notably influenced by the specific material type due to distinct frequency characteristics inherent to each material. This sensitivity stems from the distinct frequency characteristics of AEs, reflecting the microphysical processes unique to each granular material. Consequently, models trained on one material do not transfer effectively to another.

However, rapid fine-tuning of AEsNet substantially improves its performance, outperforming a similarly fine-tuned PhaseNet model pre-trained on natural earthquakes. This highlights the necessity of tailoring models to the specific features of laboratory-generated AEs, aligning with observations in transfer learning applications for natural seismicity.

In summary, our deep learning approach effectively enhances AE detection across diverse laboratory settings, enabling the creation of reliable AE catalogs that deepen our understanding of fault mechanics. This advancement facilitates the development of reliable AE catalogs, significantly contributing to the understanding of fault mechanics in controlled experimental environments.

How to cite: Scuderi, M. M., Poggiali, G., Pignalberi, F., and Mastella, G.: Readapting PhaseNet to Laboratory Earthquakes: AEsNet, a Robust Acoustic Emission Picker Illuminating Seismic Signatures of Different Fault Gouge Materials, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6730, https://doi.org/10.5194/egusphere-egu25-6730, 2025.

EGU25-7736 | ECS | Posters on site | SM2.2

Toward a Multi-Station Deep Learning Framework for Enhanced Earthquake Early Warning 

Jorge Antonio Puente Huerta, Christian Sippl, and Vaclav Kuna

Earthquake Early Warning (EEW) systems are vital for providing timely alerts in seismically active regions, potentially reducing damage and saving lives. However, achieving both rapid and reliable alerts remains a significant challenge. Recent advances in deep learning (DL) and established workflows for picking, associating, and locating events offer complementary paths to improved performance. In this work, we propose to investigate a multi-station deep learning framework that can be integrated with existing event-location pipelines or used directly to estimate ground shaking (e.g., peak ground acceleration, PGA). By fusing raw seismic waveforms with station metadata (e.g., location, sensor characteristics) in an end-to-end manner, the approach aims to capture both local site conditions and regional propagation effects. As an initial step, we will establish baseline performance using simpler neural networks (e.g., CNNs, LSTMs), then expand to more advanced models to evaluate potential gains in accuracy and speed. Preliminary findings indicate that aggregating real-time signals from multiple stations can outperform single-station methods in both alert timing and predictive reliability. Ultimately, our goal is to develop an adaptable, data-driven EEW pipeline that accommodates either direct shaking forecasts or event-based parameter estimation, enabling seamless integration into larger-scale monitoring networks and enhancing the timeliness of earthquake alerts.

How to cite: Puente Huerta, J. A., Sippl, C., and Kuna, V.: Toward a Multi-Station Deep Learning Framework for Enhanced Earthquake Early Warning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7736, https://doi.org/10.5194/egusphere-egu25-7736, 2025.

EGU25-9276 | Orals | SM2.2

Uncovering environmental and other exotic seismic sources with machine learning 

Clément Hibert, Joachim Rimpot, Camille Huynh, Charlotte Groult, Jean-Philippe Malet, Germain Forestier, Jonathan Weber, Camille Jestin, Vincent Lanticq, Floriane Provost, Antoine Turquet, and Tord Stangeland

Seismology, beyond the study of earthquakes, has become an indispensable tool for understanding environmental changes, offering unique insights into a wide range of phenomena and natural risks, from slope instabilities to glacial dynamics and hydrological hazards. However, the sheer volume and complexity of modern seismic datasets, amplified by the emergence of dense seismic networks and technologies such as Distributed Acoustic Sensing (DAS), pose significant challenges. Recent advances in Artificial Intelligence (AI) and Machine Learning (ML) have revolutionized our ability to analyze these datasets, enabling a deeper exploration of seismic data to find rare and exotic environmental seismic sources. 

Supervised learning approaches have been successfully applied to create large-scale instrumental catalogs of landslides and other environmental processes, at different  spatio-temporal scales, from short-term datasets recorded on dense local seismic stations networks, to chronicles spanning decades on seismic networks covering whole regions of the world (Alaska, Alps, Greenland). These techniques achieve high detection rates and robust classification of seismic events, even for low-magnitude or rare signals that traditional methods might overlook. Supervised learning approaches also allow us to advance our capability to estimate physical properties from seismic waves, such as the use of machine  learning to infer mass and kinematics of slope instabilities, which provide critical inputs for understanding the dynamics of these events and their associated hazards. These methodologies not only allow us to document environmental processes more exhaustively but also open up possibilities for studying poorly understood or previously undetectable seismic sources. Going beyond supervised learning, we have developed workflows based on self-supervised and unsupervised approaches to analyze continuous seismic data, uncovering unexpected patterns and revealing hidden environmental seismic sources recorded by dense seismic stations networks. Distributed Acoustic Sensing represents another frontier, turning fiber optic cables into dense seismic networks. By combining DAS with innovative AI-driven methods, we have demonstrated the potential to detect and classify low-magnitude earthquakes and anthropogenic sources, even in noisy environments, paving the way for real-time seismic monitoring on unprecedented scales.

By applying these AI-driven approaches, we are enhancing the field of environmental and exotic sources seismology, improving our ability to analyze vast seismic archives, and offering new tools to monitor, understand, and mitigate geohazards in a changing environment. This talk will highlight the latest methodological advances and showcase how they are applied to various geological and environmental contexts, from landslides, avalanches and glaciers in the Alps to fiber optic networks at different scales, underscoring the far-reaching implications of AI for seismological sources identification.

How to cite: Hibert, C., Rimpot, J., Huynh, C., Groult, C., Malet, J.-P., Forestier, G., Weber, J., Jestin, C., Lanticq, V., Provost, F., Turquet, A., and Stangeland, T.: Uncovering environmental and other exotic seismic sources with machine learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9276, https://doi.org/10.5194/egusphere-egu25-9276, 2025.

EGU25-9795 | ECS | Posters on site | SM2.2

Explainable artificial intelligence for short-term data-driven aftershock forecasts  

Foteini Dervisi, Margarita Segou, Brian Baptie, Piero Poli, Ian Main, and Andrew Curtis

The catastrophic nature of earthquakes drives the need for understanding seismic events, as well as for providing forecasts of when these are likely to occur. Due to the clustering nature of earthquakes, large magnitude events often trigger aftershocks that occur close to the mainshock in both space and time. In this study, we use a convolutional neural network to develop a data-driven spatiotemporal model to forecast next-day seismicity in an attempt to provide information that can contribute to answering one of the most pressing questions: whether a larger magnitude earthquake is to be expected after an intermediate magnitude event. We design our test to estimate expected seismicity within one day after earthquakes of magnitude four and above. We assemble a comprehensive dataset of earthquake catalogues from diverse tectonic regions to achieve a representative sample of input data and use it to create weekly spatiotemporal sequences of seismicity consisting of daily maps. Leveraging the predictive power of deep learning, our model uncovers complex patterns within this large dataset to produce next-day expected seismicity rate and magnitude forecasts in regions of interest. We use gradient-weighted class activation mapping (Grad-CAM) to provide visual explanations of the produced forecasts. We evaluate the performance of our forecasting model using data science and earthquake forecasting metrics and compare against persistence, which assumes no change between consecutive days, echoing typical experimental setups of forecasting models. Furthermore, we use a time series forecasting foundation model to generate next-day aftershock forecasts on the same dataset and compare these results against those produced by the convolutional neural network. We find that deep learning approaches are a promising solution for producing short-term aftershock forecasts, providing valuable insights that can contribute to better earthquake preparedness and response and be integrated with disciplinary statistics and physics-based forecasts.

How to cite: Dervisi, F., Segou, M., Baptie, B., Poli, P., Main, I., and Curtis, A.: Explainable artificial intelligence for short-term data-driven aftershock forecasts , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9795, https://doi.org/10.5194/egusphere-egu25-9795, 2025.

EGU25-10208 | Posters on site | SM2.2

The development of AI-based earthquake early warning system in China 

Jindong Song, Yefei Ren, Hongwei Wang, and Ruizhi Wen

China is a country prone to earthquakes. Earthquake early warning (EEW) is one of the important means to mitigate earthquake disasters. To mitigate the damage caused by destructive earthquakes, we are currently developing an artificial intelligence (AI)-based EEW system in China. By utilizing emerging technologies such as artificial intelligence and big data analysis, we have developed a complete set of methods for continuous measurement of EEW parameters based on AI. This AI-based method achieves the research goal of improving the accuracy and timeliness of EEW parameters measurement in the entire workflow of EEW system, including waveform interference elimination, earthquake event recognition, P-wave picking, magnitude estimation, seismic damage zone prediction, and so on. Presently, the offline testing results of this AI-based method on earthquake data in the Sichuan-Yunnan region of China show that the AI-based magnitude estimation reaches ±1 magnitude estimation error 4 s earlier than the existing EEW system. Meanwhile, some modules such as AI-based magnitude estimation and waveform interference elimination have been running online in the Fujian Earthquake Agency in China. In the future, China is expected to establish and improve an AI-based EEW system, and further reduce the casualties and economic losses caused by earthquakes through AI-based EEW system.

How to cite: Song, J., Ren, Y., Wang, H., and Wen, R.: The development of AI-based earthquake early warning system in China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10208, https://doi.org/10.5194/egusphere-egu25-10208, 2025.

EGU25-10901 | Posters on site | SM2.2

Machine-learning-based operational tsunami warning from light-speed elasto-gravity signals 

Quentin Bletery, Gabriela Arias, Kévin Juhel, Céline Hourcade, Andrea Licciardi, Adolfo Inza, Martin Vallée, and Jean-Paul Ampuero

Earthquake early warning (EEW) systems implemented worldwide use early seismic records of P waves to rapidly detect, locate, and estimate the magnitude (Mw) of potentially damaging earthquakes. These systems are well known to saturate for large magnitude events, which results in dramatic underestimation of the subsequent tsunamis. Alternative approaches based on different signals have been proposed to rapidly estimate the magnitude of large events, but these approaches are much slower (taking 10 to 20 minutes for first warning). Prompt elasto-gravity signals (PEGS) are light-speed gravitational perturbations induced by large earthquakes that can be recorded by broadband seismometers. They have tremendous potential for early warning but their extremely small amplitudes (on the order of 1 nm/s2) have challenged their possible operational use. We designed a deep learning approach to rapidly estimate the magnitude of large earthquakes based on PEGS. We applied this approach to the seismic networks operating in Japan, Chile, Alaska and Peru. We will present the performances obtained in these different contexts. In Alaska, the approach has proven capable to reliably estimate the magnitude of Mw ≥ 7.6 earthquakes (without saturation) in less than 2 minutes, outperforming state-of-the-art tsunami early warning algorithms. Motivated by these performances, we initiated a first implementation of an operational tsunami warning system based on PEGS in Peru. We will present the simulated real-time performance of this system. 

How to cite: Bletery, Q., Arias, G., Juhel, K., Hourcade, C., Licciardi, A., Inza, A., Vallée, M., and Ampuero, J.-P.: Machine-learning-based operational tsunami warning from light-speed elasto-gravity signals, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10901, https://doi.org/10.5194/egusphere-egu25-10901, 2025.

EGU25-11335 | ECS | Orals | SM2.2

Unsupervised Clustering and Pattern Identification from Continuous Seismic and Strainmeter Data in Tectonic and Volcanic Settings 

Zahra Zali, Patricia Martínez-Garzón, Grzegorz Kwiatek, Gregory Beroza, Fabrice Cotton, and Marco Bohnhoff

We developed a deep learning model for automatic dimensionality reduction and feature extraction from time series. The model employs an encoder-decoder architecture with skip connections, enabling efficient compression and reconstruction of input data while preserving essential features. These features are used for unsupervised clustering enabling anomaly detection, and pattern recognition.

We initially developed the model to analyze seismic data from the 2021 Geldingadalir volcanic eruption in Iceland, successfully identifying a weak yet important pre-eruptive tremor that commenced three days before the eruption. Advancing the architecture with additional layers and skip connections allowed for highly accurate input reconstruction. The latter version, named AutoencoderZ, demonstrated its ability to process different data types. We applied AutoencoderZ to investigate low-frequency patterns preceding the 2023 MW 7.8 Kahramanmaraş Earthquake in Türkiye. The model identified tremor-like episodes linked to anthropogenic activities at cement plants near the earthquake’s epicenter. Additionally, we applied AutoencoderZ to strainmeter data from the Sea of Marmara, achieving accurate reconstructions and enabling the detection of distinct tectonic-related signals.

This study highlights AutoencoderZ’s potential as a powerful tool for uncovering patterns in continuous geophysical data, providing valuable insights for monitoring and interpreting seismic and strainmeter signals.

How to cite: Zali, Z., Martínez-Garzón, P., Kwiatek, G., Beroza, G., Cotton, F., and Bohnhoff, M.: Unsupervised Clustering and Pattern Identification from Continuous Seismic and Strainmeter Data in Tectonic and Volcanic Settings, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11335, https://doi.org/10.5194/egusphere-egu25-11335, 2025.

EGU25-11459 | ECS | Posters on site | SM2.2

Automating Seismic Event Discrimination: A Comparative Study of Convolutional Neural Networks and Vision Transformers 

Valentin Kasburg, Marcel van Laaten, Markus Zehner, Jozef Müller, and Nina Kukowski

To date, the discrimination of seismic events recorded in seismic networks is often performed manually by experts, classifying events into categories such as earthquakes, quarry blasts, or mining events. While recent studies have shown that deep learning algorithms, particularly Convolutional Neural Networks (CNNs), can efficiently and accurately distinguish between different types of seismic events, their application for automated seismic event discrimination remains limited. This limitation arises from several factors, including the absence of globally applicable models that maintain high precision for local seismic networks, the scarcity of data required for fine-tuning Deep Learning (DL) models, and the lack of interpretability in the decision-making processes of these black-box models.

In this contribution, we explore the use of Vision Transformers (ViTs) as a novel approach for automating seismic event discrimination. To assess their potential for accuracy and explainability, we applied CNNs and ViTs to classify seismic events such as earthquakes, quarry blasts, and mining events. For this purpose, we pretrained the models on openly available seismic event data from Utah and Northern California and then fine-tuned and tested them on data from the Seismic Network of the Ruhr-University Bochum (RuhrNet) and the Thuringian Seismic Network (TSN).

Our findings reveal that ViTs can analyze the entire spectrogram of a seismic event in a coherent manner, offering superior generalizability in pattern recognition compared to CNNs. In addition to achieving high discrimination accuracy, the attention weights of ViTs provide insights into the models’ decision-making process, offering a transparent and interpretable explanation of the underlying mechanisms driving its classifications.

How to cite: Kasburg, V., van Laaten, M., Zehner, M., Müller, J., and Kukowski, N.: Automating Seismic Event Discrimination: A Comparative Study of Convolutional Neural Networks and Vision Transformers, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11459, https://doi.org/10.5194/egusphere-egu25-11459, 2025.

EGU25-13238 | ECS | Orals | SM2.2

A Waveform-Based Graph Neural Network Approach for Microseismic Monitoring 

Matteo Bagagli, Francesco Grigoli, and Davide Bacciu

In this work, we introduce HEIMDALL, a grapH-based sEIsMic Detector And Locator specifically designed for microseismic applications. Building on recent progress in deep learning (DL), HEIMDALL employs spatiotemporal graph-neural networks to detect and locate seismic events in continuous waveforms. It simultaneously associates and provides preliminary locations by leveraging the output probability functions of the graph-neural network over a dense, three-dimensional grid (0.1 km spacing). By integrating detection and location within a single framework, HEIMDALL aims to address persistent challenges in microseismic data analysis, such as accurately associating wavefront arrivals and enabling consistent and robust event localization in complex geothermal regions. To train our models, we utilize synthetics generated using Green’s function available in the area, in combination with a small fine-tuning over a subset of real data. This approach allows us to achieve homogeneous coverage of the study area while addressing nuances that inevitably arise across synthetic and real domains.

Our evaluation focuses on data collected at the Hengill Geothermal Field in Iceland as part of the COSEIMIQ project (December 2018 to August 2021). Specifically, we analyzed one month of continuous seismic recordings from December 2018 and a brief sequence on February 3, 2019, which occurred in the middle of the geothermal plant. The dataset also features frequent burst sequences, providing an ideal testbed for advanced detection and location algorithms. By benchmarking HEIMDALL against multiple approaches, we reveal both the strengths and limitations inherent in our novel method and in more conventional workflows used in observational seismology.

Ultimately, we highlight the importance of continued innovation in ML-based workflows for induced seismicity monitoring at enhanced geothermal system (EGS) sites, where the capacity to detect and accurately locate a large number of microseismic events can be critical for operational safety and resource management.

How to cite: Bagagli, M., Grigoli, F., and Bacciu, D.: A Waveform-Based Graph Neural Network Approach for Microseismic Monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13238, https://doi.org/10.5194/egusphere-egu25-13238, 2025.

EGU25-13430 | ECS | Posters on site | SM2.2

Towards the robust Clustering of various cryogenic signal types using Seismic Array Information 

Antonia Kiel, Vera Schlindwein, and Conny Hammer

Ice mass loss in polar regions is a major contributor to sea level rise driven by climate change. To better predict ice mass loss due to calving and melting, it is essential to monitor ice dynamics by linking observed seismic signatures to physical processes such as meltwater infiltration into crevasses or crack formation caused by high tides at the grounding line. However, current knowledge about the distinct patterns of icequake types remains limited.

To address this gap, approximately 15 years of continuous seismic data from the Watzmann Array near the Neumayer Station in Antarctica are analyzed to automatically cluster seismic recordings. This analysis involves the automatic extraction of seismic events and the application of beamforming to each event. As a result, directional information is incorporated and the local noise is significantly reduced.

In the following, clustering methods, combined with techniques like dynamic time warping and feature extraction, are employed to categorize seismic events into distinct groups representing different icequake types. A key focus of this work is on leveraging dynamic time warping to cluster seismic waveforms directly, prioritizing the identification of physical properties inherent in the signals rather than relying solely on features extracted through machine learning. This approach ensures that the obtained clustering reflects the true underlying source processes rather than being limited to abstract feature representations.

In a follow-up study, these clusters can be related to environmental factors and directional information. Finally, with this we hope to shed some light on the hidden source processes of observed icequake types.

How to cite: Kiel, A., Schlindwein, V., and Hammer, C.: Towards the robust Clustering of various cryogenic signal types using Seismic Array Information, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13430, https://doi.org/10.5194/egusphere-egu25-13430, 2025.

Recent advances in machine learning (ML) have enabled significant progress in geoscience by capturing complex relationships and enhancing predictive skills. However, the success of many ML algorithms in data-rich settings does not seamlessly transfer to climate and atmospheric applications, where observational datasets are often limited. This underscores the need for methods that deliver high predictive accuracy under data-scarce conditions while retaining interpretability.

Here, we compare various ML approaches with the Nonlinear AutoRegressive Moving Average model with eXogenous inputs (NARMAX) in typical small-data climate applications, such as seasonal weather forecasting and Greenland Blocking Index (GBI) prediction. NARMAX, a transparent, interpretable, parsimonious and simulatable (TIPS) framework, demonstrates robust performance and avoids common pitfalls such as overfitting and unstable predictions when data are scarce. Notably, it achieves superior or competitive forecast accuracy for small or limited data conditions, underscoring its practical value in operational climate science. By adopting a sparse system identification approach, NARMAX yields model structures that readily reveal key predictors and their relative contributions, providing valuable physical and statistical insights into climate variability.

Our findings illustrate how NARMAX bridges the gap between purely data-driven modelling (focusing on prediction) and mechanistic modelling (focusing on physical insights), offering a clear pathway for refining model strategies and deepening our understanding of climate dynamics. We propose that NARMAX and similar methods play an inherently powerful role for both small and large data modelling problems and meanwhile serve as potent components to potentially improve the explainability of ML methods. By showcasing both interpretability and predictive efficacy, this work encourages the adoption of machine learning methods that best meet the needs for specific data modelling tasks in climate science and beyond.

How to cite: Sun, Y., Wei, H.-L., Hanna, E., and Luu, L.: Small Data for Big Tasks in Seasonal Weather Forecasting: A Balanced Perspective on Interpretability and Predictability of NARMAX and Machine Learning Methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13666, https://doi.org/10.5194/egusphere-egu25-13666, 2025.

Substorms are a magnetospheric phenomenon which causes high geomagnetic and auroral disturbances. It is widely accepted that substorm activity is controlled by solar wind conditions. It is, however, difficult to predict substorms deterministically because of the complex physical processes underlying substorm occurrences. We propose a framework for modelling time series of event occurrences controlled by external forcing. In this framework, occurrences of external-driven events are represented with a non-stationary Poisson process, and its intensity, which corresponds to the occurrence rates per unit time, is described with a simple machine learning model, the echo state network, which is fed with forcing variables. The echo state network is trained by maxmising the likelihood given the event time series data. 

We apply this approach for analysing time series of substorm onsets identified from Pi2 pulsations, which are irregular geomagnetic oscillations associated with substorm onsets. We train the echo state network to well describe the response of substorm activity to solar-wind conditions. We then examine the characteristics of the substorm activity by feeding synthetic solar-wind data into the echo state network. The results show what solar wind variables effectively contribute to the substorm occurrence. 

Our echo state network model is also useful for examining the statistical properties of the substorm occurrence rate. For example, we can evaluate what mainly controls the seasonal and UT variations of substorm activity. There are two explanations for the seasonal and UT variations. One explanation is that the seasonal and UT variations is controlled by the inner product between the solar-wind magnetic field and the Earth's dipole axis. The other is that the variations are due to the angle between the solar-wind flow and the Earth's dipole axis. Since these two effects are related with different input variables in our echo state network model, we can examine the contribution of each effect to the substorm occurrence frequency. The result shows that the seasonal and UT variations are mostly dependent on the angle between the solar-wind flow and the Earth's dipole axis. 

How to cite: Nakano, S., Kataoka, R., and Nose, M.: Modelling of time series of external-driven events with echo state network and its application to substorm activity analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14041, https://doi.org/10.5194/egusphere-egu25-14041, 2025.

EGU25-14779 | ECS | Posters on site | SM2.2

Deep Learning-Based Surface-Related Multiple Suppression in Shallow Arctic Seismic Data 

Hyeji Chae, Daeun Na, Seung-Goo Kang, and Wookeen Chung

Seismic data recorded in shallow water in the Arctic Ocean contain not only primary reflections but also surface-related multiples with strong amplitudes and short-period characteristics. These multiples generate false stratigraphic boundaries on stacked seismic sections, thereby reducing the accuracy of geological interpretation. Therefore, the attenuation of multiples is an essential step in seismic data processing for accurate geological interpretations. Recently, with the advancement of deep learning technology, research on suppressing surface-related multiples using deep learning networks (such as U-Net and stacked BiLSTM) has been actively proposed.

Firstly, surface-related multiple suppression algorithms using U-Net and stacked BiLSTM were applied to Arctic field data respectively. Each algorithm was designed to predict surface-related multiples by using input data that contained both primary reflections and surface-related multiples. Fractional Fourier transform (FrFT) and continuous wavelet transform (CWT), which represent time-series data in the time-frequency domain, were applied to synthetic data and used as input data feature for each network. Finally in order to suppress the surface-related multiples for seismic data in shallow depth Arctic Ocean, the proper methods (network architectures, input data feature) are suggested.

 

Acknowledgments

This research was supported by Korea Institute of Marine Science & Technology Promotion (KIMST) funded by the Ministry of Oceans and Fisheries, Korea (RS-2023-00259633).

 

How to cite: Chae, H., Na, D., Kang, S.-G., and Chung, W.: Deep Learning-Based Surface-Related Multiple Suppression in Shallow Arctic Seismic Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14779, https://doi.org/10.5194/egusphere-egu25-14779, 2025.

EGU25-15039 | ECS | Posters on site | SM2.2

Machine learning and feature extraction for detecting transient signals in GNSS time series 

Martín Sepúlveda, Marcos Moreno, and Matthew Miller

Advances in the processing of Global Navigation Satellite System (GNSS) positioning data and the increasing densification of geodetic networks have provided an unprecedented opportunity to detect and analyse transient deformation signals, including Slow Slip Events (SSE). These events, characterised by very slow rupture and durations of days to months, are often associated with areas of low coupling and sometimes show clear recurrence patterns. Despite their importance in subduction zones, reliable detection of SSEs remains an ongoing challenge. The sheer volume of GNSS data, combined with high noise levels and the subtle nature of these signals, requires efficient and robust methods capable of rapidly processing large datasets.

To overcome these challenges, we propose a method that relies on feature extraction techniques and machine learning to improve the detection and analysis of possible SSEs. Specifically, we use the TSFRESH algorithm to extract relevant features from GNSS time series, coupled with supervised machine learning classification techniques. Preliminary results of our current model, trained on synthetic data and validated through various performance tests, demonstrate high detection capabilities and accuracy. We further validated the model using a collection of GNSS time series from the Cascadia subduction zone with a single-station method scaled to the entire network, where the model showed satisfactory performance in detecting possible SSEs compared to similar work. Future efforts will focus on improving the robustness and generalisation of the model to new data, and refining methods for estimating the slip and duration of each possible SSE.

How to cite: Sepúlveda, M., Moreno, M., and Miller, M.: Machine learning and feature extraction for detecting transient signals in GNSS time series, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15039, https://doi.org/10.5194/egusphere-egu25-15039, 2025.

EGU25-15129 | ECS | Posters on site | SM2.2

Auto-Picking of First-Break Refractions in Arctic Ocean Seismic Data Using Stacked BiLSTM Networks 

Seoje Jeong, Hyeji Chae, Seung-Goo Kang, Sung-Ryul Shin, and Wookeen Chung

 In seismic exploration data from the Arctic Ocean, refractions are recorded earlier than direct waves due to the shallow depths and subsea permafrost with high velocity. These refraction signals could be utilized for estimating the velocity, thickness, and depth of the subsea permafrost. However, it is very challenging work to pick the accurate first arrivals of seismic data in the Arctic Ocean because of many factors such as ambient noise and etc. Therefore, identifying first-break refractions is crucial and can be performed by manual or automated picking methods. Various semi-automatic techniques have been developed to identify first-break refractions, but these methods are often sensitive to pulse variations and require parameter tuning. Recently, deep learning-based methods have also been explored, but their reliance on training data often results in inconsistent performance, making it essential to generate training data optimized for the target environment. 

This study presents a recurrent neural network-based algorithm optimized for Arctic Ocean environments to automatically identify first-break refractions. To effectively classify first-break refractions, a stacked bidirectional long short-term memory (BiLSTM) network was constructed to iteratively learn bidirectional long-term dependencies by utilizing the temporal patterns of time-series data. Additionally, the training data were generated by creating velocity models that reflect the subsurface properties of subsea permafrost, enabling the generation of first-break refraction label data. The proposed network demonstrated superior performance in identifying first-break refractions from noisy data, achieving over 95% accuracy in numerical experiments and field tests. Field data applications demonstrated that the proposed network achieves high accuracy in classifying first-break refractions, validating its robustness and adaptability.

 

 

Acknowledgments

This research was supported by Korea Institute of Marine Science & Technology Promotion (KIMST) funded by the Ministry of Oceans and Fisheries, Korea (RS-2023-00259633).

How to cite: Jeong, S., Chae, H., Kang, .-G., Shin, .-R., and Chung, W.: Auto-Picking of First-Break Refractions in Arctic Ocean Seismic Data Using Stacked BiLSTM Networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15129, https://doi.org/10.5194/egusphere-egu25-15129, 2025.

EGU25-16157 | ECS | Posters on site | SM2.2

Real Time Estimation of Earthquake Location and Magnitude Using Large Language Models 

Aurora Bassani, Daniele Trappolini, Giulio Poggiali, Elisa Tinti, Fabio Galasso, Chris Maron, and Alberto Michelini

Estimation of earthquake parameters has always been a focus for seismologists. Efficient and rapid determination of earthquake location and magnitude is essential for mitigating the potential hazards associated with seismic shaking. Nowadays, Earthquake Early Warning Systems (EEWS) are implemented in most earthquake-prone areas, with the system varying according to the specific needs. Although methods for their estimation exist, many still lack a fast enough process, which is crucial for reducing the waiting time before issuing a warning.

Here, we propose a novel model to enhance multi-station EEWS using Large Language Models (LLM). We adopt a pre-trained LLM and fine-tune it on a customized version of INSTANCE (The Italian Seismic Dataset for Machine Learning), thus eliminating the need to develop and train a tailor-made architecture. The model uses stations with P-wave arrival times up to 5 s apart from the first recorded one, and, for each seismic trace, it exploits a very small time window around the P-wave arrival time (0.21 s), thus effectively reducing warning latency.

Comparative analysis against the automatic method employed by the Italian National Institute of Geophysics and Volcanology (INGV) demonstrates that our model achieves comparable performance in magnitude estimation and superior accuracy in epicenter, hypocenter and origin time prediction. For instance, the LLM-based model achieves average errors of 6.3 km, 11.1 km, and 1.1 s for epicenter, hypocenter, and origin time estimation, respectively, in contrast to 8.6 km, 15.0 km, and 1.8 s for the INGV automatic solution resulting in an average improvement of more than 26% for all parameters.

We study the validity of our model by assessing its ability using P- and S-waves to predict magnitude, and show that in this case study the S-waves are not strictly necessary for accurate predictions.

How to cite: Bassani, A., Trappolini, D., Poggiali, G., Tinti, E., Galasso, F., Maron, C., and Michelini, A.: Real Time Estimation of Earthquake Location and Magnitude Using Large Language Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16157, https://doi.org/10.5194/egusphere-egu25-16157, 2025.

EGU25-17400 | ECS | Orals | SM2.2

Deep learning to investigate post-seismic evolution of fault zone elastic properties 

Gabriele Paoletti, Daniele Trappolini, Elisa Tinti, Fabio Galasso, Cristiano Collettini, and Chris Marone

Fault zone properties evolve dynamically during the seismic cycle due to stress changes, microcracking, and wall rock damage. Understanding these changes is vital to gaining insights into earthquake preparation and post-seismic processes. The latter include fault healing, which refers to the recovery of mechanical and elastic properties in fault zones after seismic and aseismic fault slip. Despite its importance, detecting and characterizing fault healing through seismic signals remains a challenge due to the subtle nature of these changes.

In this study, we investigate the potential of deep learning techniques, specifically a 4-layer Convolutional Neural Network (CNN), to characterize post-seismic evolution by analyzing raw seismic waveforms recorded after the largest event (Mw 6.5,  30 October) of the 2016 Central Italy seismic sequence. These data provide a unique opportunity to examine fault zone dynamics. A key aspect of our approach is the hypothesis that ray paths traversing highly impacted areas of the fault zone contain richer information about its temporal evolution. To test this hypothesis, we examined seismic waves from two clusters — DHwS, located in the hanging wall beneath the hypocentral region, and C1, situated in the footwall. They represent contrasting ray trajectories as recorded on seismic stations MC2 and MMO1. Seismic waves recorded at MC2 pass through heavily damaged fault regions, which are likely to reveal evolving fault properties, whereas MMO1 predominantly captures paths that skirt or in the case of C1 completely miss these impacted areas, serving as a comparative baseline.

We assessed temporal variations in elastic properties using binary classification tests on normalized, raw seismic waveforms of events before and after a reference date. This date was arbitrarily selected within the temporal range of the analyzed seismicity and serves solely as a neutral point of comparison. Our hypothesis is that if the CNN can achieve good classification performance, it implies the presence of time-evolving properties in the fault zone, potentially linked to healing processes or other time-dependent factors.

To further validate these findings, we employed adversarial training, a technique designed to disentangle time-dependent effects from structural changes. By introducing controlled label noise into one cluster during training, we isolated the influence of confounding factors such as seasonal variations. Preliminary results suggest that adversarial training enhances the model's robustness and provides valuable insights into the time-evolving properties of the fault zone.

Deep learning offers significant potential for analyzing spatiotemporal changes in elastic properties and thus the evolution of fault zone properties over the seismic cycle. By detecting subtle temporal and structural changes, we hope to gain a deeper understanding of fault dynamics and post-seismic processes.

How to cite: Paoletti, G., Trappolini, D., Tinti, E., Galasso, F., Collettini, C., and Marone, C.: Deep learning to investigate post-seismic evolution of fault zone elastic properties, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17400, https://doi.org/10.5194/egusphere-egu25-17400, 2025.

EGU25-19236 | ECS | Orals | SM2.2

High Resolution Generative Waveform Modeling Using Denoising Diffusion 

Kadek Hendrawan Palgunadi, Andreas Bergmeister, Andrea Bosisio, Laura Ermert, Maria Koroni, Natanaël Perraudin, Simon Dirmeier, and Men-Andrin Meier

Reliable synthesis and prediction of seismic waveforms play an important role in evaluating seismic hazards and designing earthquake-resilient structures. However, current methods, such as ground motion models and physics-based simulations, are often limited in fully capturing the complexity of seismic wave propagation, at higher frequencies (>5 Hz). Some of these limitations can potentially be overcome through machine learning techniques. In earthquake engineering, machine learning models have been used for predicting peak ground accelerations and Fourier spectra responses. To model entire waveforms, extensive efforts to generate seismic waveforms have employed advanced machine learning techniques, such as generative models, with most previous approaches relying on generative adversarial networks (GANs). In contrast to these earlier models, this study presents an efficient and extensible generative framework to produce realistic high-frequency seismic waveforms, compared to GANs. Our approach encodes spectrograms of the waveform data into a lower-dimensional sub-manifold using an autoencoder, and a state-of-the-art diffusion model is subsequently trained to generate these latent embeddings. Conditioning is currently performed on key parameters: earthquake magnitude, recording distance, site conditions, and faulting style. The resulting generative model can synthesize waveforms with frequency content up to 50 Hz, from which several scalar ground motion statistics, such as peak ground motion amplitudes, spectral accelerations, or Arias intensity can be directly derived. We validate the quality of the generated waveforms using standard seismological benchmarks and performance metrics from image generation research. Our openly available model produces high-frequency waveforms that align with real data across a wide range of input parameters, including regions where observations are sparse, and accurately reproduces both median trends and variability of empirical ground motion statistics. Our generative waveform model can be potentially used to perform seismic hazard where broadband data are often required such as to train earthquake early warning model. Given the increasing number of generative waveform models, we emphasize that they should be openly accessible and included in community efforts for ground motion model evaluations.

How to cite: Palgunadi, K. H., Bergmeister, A., Bosisio, A., Ermert, L., Koroni, M., Perraudin, N., Dirmeier, S., and Meier, M.-A.: High Resolution Generative Waveform Modeling Using Denoising Diffusion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19236, https://doi.org/10.5194/egusphere-egu25-19236, 2025.

EGU25-21456 | Orals | SM2.2

Prediction of measured earthquake waveforms from synthetic data: a two-step deep learning approach 

Alexander Bauer, Jan Walda, and Conny Hammer

Single-station waveforms of teleseismic earthquakes are highly complex, because they are a superposition of numerous phases corresponding to different wave types and propagation paths. Moreover, data recorded at single stations is contaminated by noise, which often has similar or larger amplitudes than the arrivals of teleseismic earthquakes, especially in densely-populated areas. For high precision research facilities, for example in the field of particle physics or gravity wave detection, a precise knowledge of the seismic wavefield generated by teleseismic earthquakes can be critical for the calibration of experiments. However, the density of seismological stations is often sparse, particularly in regions with low seismic hazard such as Northern Germany.

To overcome this limitation, we introduce a deep learning scheme for the prediction of very-low-frequency earthquake waveforms from synthetic data at arbitrary locations within the metropolitan area of Hamburg, Germany. For this aim, we propose to train a convolutional neural network (CNN) to predict the measured earthquake waveforms from their synthetic counterparts. While synthetic earthquake waveforms can be conveniently generated for arbitrary coordinates and moment tensors with Instaseis and the IRIS synthetics engine (Syngine), the amount of available measured waveforms is constrained by the availability of seismological stations and their installation date. In this work, we use measured data from a station in Bad Segeberg, north of Hamburg, which has been measuring continuously since 1996. During first experiments, we trained a CNN on data from earthquakes larger than M6.0 and obtained reasonable initial results. However, the number of such earthquakes is limited and the measured waveforms used as labels partly contained noise of considerable amplitude, which caused the neural network to predict unwanted noise.

In order to increase the amount of earthquakes in the training data and mitigate their contamination with noise, we propose a two-step approach. In the first step, we generate a large number of noise-free synthetic waveforms and contaminate them with artificially generated noise that has the same characteristics as the noise measured at the station in Bad Segeberg. With this dataset, we train a first CNN to denoise the synthetic earthquake waveforms. In the second step, we apply the trained neural network to the actual earthquake waveforms measured in Bad Segeberg to denoise them. We then train a second CNN to translate synthetic earthquake waveforms to the denoised measured ones. Results for earthquakes not part of the training data demonstrate that the second CNN provides convincing estimates of measured earthquake waveforms, not only for the station in Bad Segeberg, but also for stations in Hamburg. This can be seen as a first step towards a three-dimensional prediction of the earthquake wavefield without the need for densely-distributed stations.

How to cite: Bauer, A., Walda, J., and Hammer, C.: Prediction of measured earthquake waveforms from synthetic data: a two-step deep learning approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21456, https://doi.org/10.5194/egusphere-egu25-21456, 2025.

EGU25-275 | ECS | Orals | GI2.4

Application of Machine Learning Algorithms to Predict Rock Types Using Geochemical Data: A Case Study from the Obuasi Gold District, Ghana 

Abdullah Bello Muhammed, Emmanuel Daanoba Sunkari, and Abdul Wahab Basit

Artificial Intelligence and Machine Learning (AI/ML) are gaining increasing interest due to their capacity to increase precision and productivity in the current big data era. Machine learning has indicated its robustness in geosciences, particularly rock-type classification. Lithological classification in the traditional way has raised critical concerns and the need to curb the limitations it breeds, such as time consumption and subjective results. The gold mineralisation occurrence is structurally controlled in the Obuasi Gold district of Ghana. It exhibits complex patterns and relationships that may not be readily discernible through traditional methods, leading to missing out on discovering new resources or potential exploration targets. Consequently, this work attempts to create a predictive model by exploring the best machine-learning algorithms to predict rock types in the Obuasi Gold District using X-ray fluorescence (XRF) geochemical data. Here we established comparative predictive modelling using four supervised classification algorithms: Gradient Boosting (GBoost), Adaptive Boosting (AdaBoost), Support Vector Machine (SVM) and Random Forest (RF). The acquired XRF data was integrated with the model using the Google Collaboratory cloud-based platform. Results show that the performance evaluation of the models indicated SVM as the best algorithm for deployment with a Classification Accuracy (CA) of 0.902. Therefore, ML algorithms have been a great tool in rock-type classification, whereby SVM emerged as the best in the case of the Obuasi Gold District. However, it is encouraged to understand the geology of a particular area before employing the tool and the datasets must be balanced to yield good results and avoid model overfitting.

Keywords: Artificial intelligence; Machine learning algorithm; Support vector machine; Lithogeochemistry; Rock-type classification; Obuasi Gold District

How to cite: Muhammed, A. B., Sunkari, E. D., and Basit, A. W.: Application of Machine Learning Algorithms to Predict Rock Types Using Geochemical Data: A Case Study from the Obuasi Gold District, Ghana, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-275, https://doi.org/10.5194/egusphere-egu25-275, 2025.

Preserving clean water resources and efficiently treating wastewater is critical for ensuring human survival on Earth and in extraterrestrial environments. Major pollutants, including ammonium, heavy metals, industrial dyes, and chemicals, threaten limited clean water supplies and soil. Among the renowned absorbent materials, natural zeolite minerals have demonstrated their effectiveness for pollutant removal compared to clay minerals and synthetic equivalents like biochar, activated carbon, and MOFs, owing to their relatively extensive reserves and eco-friendly nature. Recently, investigating and optimizing pollutant removal rates from water without conducting laboratory experiments is getting more crucial, considering the time-consuming, expensive, and error-prone nature of laboratory testing due to human factors and potential calibration issues among the chosen analytical techniques.

This study aims to forecast the ammonium removal efficiency (% adsorption) and capacity (mg/g) of natural and modified zeolites from aqueous solutions using the regression ensemble LSBoost (MATLAB R2024b) machine learning (ML) algorithm, which is equivalent to XGBoost open-source library. A total of 527 experiments on 15 different zeolite compositions were gathered from a combination of 14 suitable moderately recent (≥ 2005) and highly referred studies to assess the performance of zeolite minerals on ammonium removal rates from aqueous solutions. The LSBoost algorithm achieved over 0.99 R2 fitting for training and overall, 0.95 R2 for prediction on the quarterly partitioned testing data for both efficiency and capacity. Throughout the improvement of the ML models using different random forest ML approaches, the number of predictors was successfully reduced to 8 based on importance rates among 31 different features in the initial dataset, with a negligible accuracy loss (<0.1 R2) on both training and testing. This research provides a valuable contribution to optimizing applicable experimental parameters in water treatment processes by effectively identifying the significance of predictors within a comprehensive data set. In addition to this, our model not only provides a robust predictive tool for optimizing zeolite performance in water treatment but also represents the first open-sourced web application in the literature to estimate the water treatment performance of zeolites.

How to cite: Akkaş, E., Ünal, B. C., and Ersoy, O.: AI-Based Prediction and Optimization of Ammonium Removal Efficiency and Capacity of Natural Zeolites Using LSBoost (XGBoost) for Sustainable Ecosystems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-809, https://doi.org/10.5194/egusphere-egu25-809, 2025.

EGU25-882 | ECS | Orals | GI2.4

Assessment of a deep learning framework for time-lapse seismic monitoring 

Giovanni Pantaleo and Michele Pipan

In the context of CO₂ storage, cost-effective monitor methods are essential to ensure safe and long-term storage. This work explores the use of seismic time-lapse monitoring, combined with deep learning (DL) techniques, to assess potential leakage and migration pathways. The goal is to develop a cost-effective monitoring method while guaranteeing the safety of storage operations. To this end, we propose a Siamese Neural Network (SNN)-based framework to analyse shot gathers, designed to detect and localize changes within the storage complex. We aim to address the challenges of working with large seismic datasets, enabling the identification of significant events with high confidence, while avoiding the need for event-by-event processing. This framework can allow experts to rely on semi-automatic detections while ensuring human evaluation for interpreting and validating the results.

The proposed SNN architecture processes pairs of shot gather from baseline and monitor surveys in a cross-well configuration. It uses two identical neural networks with shared weights to encode the shot gathers into latent feature embeddings, which are then compared to identify similarities and detect changes. By transforming the data into a shared latent space, the model focuses on capturing relevant patterns while filtering out irrelevant variations, ensuring robust and accurate comparisons. When the SNN detects changes between the baseline and the monitor surveys, it highlights the regions where these changes occur. This approach is particularly effective for identifying subtle but important changes in seismic data, such as those caused by CO₂ migration, which alters the velocity and density of the subsurface. Even in noisy data, the SNN can detect these variations, thanks to its ability to learn features that are highly sensitive to small but meaningful changes. The SNN architecture is scalable and can be adaptable to various seismic monitoring tasks, requiring minimal preprocessing. The proposed framework harnesses the power of deep learning to provide insights into the dynamics of the storage complex, with a focus on identifying changes in time-lapse seismic data related to localized variations. The proposed migration detection tool offers a cost-effective and reliable solution to the modern challenges of gas storage monitoring. This study aims to enable operators to identify and address problems promptly, thereby minimising the impact of potential leakages.

How to cite: Pantaleo, G. and Pipan, M.: Assessment of a deep learning framework for time-lapse seismic monitoring, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-882, https://doi.org/10.5194/egusphere-egu25-882, 2025.

Joint inversion is an essential technique in potential field data processing. The current methodology largely relies on the geology model of anomalous bodies, especially for deep, complex structures. Inspired by the excellent nonlinear mapping capability of the image semantic segmentation model and the advantages of supervised learning, a regressive, end-to-end, encoder-decoder structural, convolutional neural network with a double-branch structure called PFInvNet(Potential Field Inversion Neural Network) is proposed for joint 3D  inversion of physical properties from gravity and magnetic data. Its input is a four-channel dataset consisting of gravity and magnetic anomalies and their vertical gradients, and its output is a 3D matrix representing the spatial distribution of the remnant density and the magnetic susceptibility, which are predicted independently through the double-branch structure of the decoders and then concatenated in the final layer. For network training, a large amount of precisely labeled sample is exceedingly demanding; thus, forward modeling becomes a prerequisite approach. Two discretized forward modeling algorithms for gravity and magnetic anomalies of 3D homogeneous arbitrary-shaped bodies based on surface integrals are deduced and verified with analytic solutions of the sphere model. Furthermore, the neural network needs to learn from the anomalies generated by various forms of abnormal bodies with different physical properties. Therefore, different sizes and quantities of cuboids are randomly distributed in the model space to simulate different forms of abnormal bodies. The label represents the combined spatial distribution of remanent density and magnetic susceptibility for the cuboids, encompassing both spatial location information and physical properties information. With the help of the Marching Cubes(MC) algorithm, the surface of the cuboids can be easily extracted and divided into a triangular surface mesh. The surface mesh is then used to calculate the gravity and magnetic anomalies synchronously through the forward modeling algorithms. The anomalies are concatenated in the channel direction as a sample. A set of optimal network parameters has been determined, including the weight initialization method, the gradient calculation methods, the loss function, the training hyperparameters, the regularization method, and the normalization method. The PFInvNet is trained with 500 and 10000 pairs of samples and labels, respectively. The analysis and comparison of training results prove that PFInvNet has two crucial features: one is that the branch structure enables independent prediction of magnetic susceptibility and remanent density; the other is efficient anti-overfitting ability and efficient solution-finding ability .The prediction error of small samples is very close to that of large samples and is also not obviously enhanced by the noise-contaminated data , demonstrating the strong generalization and robustness of the network. Finally, the network is tested with magnetic and gravity anomalies of the Victoria Land Basin in the western Ross Sea through transfer learning and retraining, and definite 3D distributions of apparent remnant density and apparent magnetic susceptibility have been obtained and can be checked with geological evidences.

How to cite: Jiang, W., Zhao, Y., Gao, J., Ge, S., and Xie, Z.: 3D property inversion of gravity and magnetic data based on a double branch regressive CNN trained by synchronous forward modeling :a case study of the Western Ross Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1141, https://doi.org/10.5194/egusphere-egu25-1141, 2025.

EGU25-2156 | ECS | Orals | GI2.4

TOC Intelligent Prediction Model in Shale Reservoir: Integrating Data Enhancement with Empirically Driven Algorithm 

Yuzhen Hong, Shaogui Deng, Zhijun Li, and Zhoutuo Wei

Shale oil and shale gas are important unconventional resources. Organic matter serves as the primary source of shale oil and gas generation, and high TOC values typically indicate better oil and gas reservoir conditions and production. Therefore, an accurate TOC prediction model is conducive to low-cost evaluation of reservoir hydrocarbon potential and improvement of development efficiency. However, geochemical experimental measurements are costly, and the data obtained is discrete. It is unable to meet the requirements for fine-scale assessment of shale reservoirs. The multiple regression method and ΔlogR method, when directly applied to shale reservoirs, often result in significant errors. In this study, we propose a composite model for accurate TOC prediction in shale reservoirs based on data enhancement and empirically driven. We first address the issue of poorly characterized logging responses and discrete experimental data. The features and quantities of the dataset are enhanced by introducing reconstruction curves and generative adversarial networks (GAN). The validity of the synthesized data is then verified by plotting the data density. In the empirically-driven module, we optimize a density-gamma modified method on traditional ΔlogR method according to the characteristics of shale reservoirs. The modified ΔlogR method will be integrated into the GWO-SVR model as an empirically driven subject in the form of a fitness function. Above, a composite model with both empirical and data-driven components is constructed. We use the Dongying Depression in China as an example for model experiments. The composite model was generalized to wells X and Y. The R² (coefficient of determination) was 0.95 and 0.97, the RMSE (Root Mean Square Error) was 0.31 and 0.29, and the MAE (Mean Absolute Error) was less than 0.3, which indicated a high degree of consistency between the model predictions and the experimental values. Further controlled experiments revealed that the composite model predicted better than the ΔlogR method and the GWO-SVR model alone. Finally, we also performed SHAP interpretability analysis on the model. By revealing the decision-making mechanism inside the model, we verified the rationality of the empirical drive and enhanced the credibility of the model. This provides strong technical support and decision-making basis for the subsequent oil and gas exploration and development work.

How to cite: Hong, Y., Deng, S., Li, Z., and Wei, Z.: TOC Intelligent Prediction Model in Shale Reservoir: Integrating Data Enhancement with Empirically Driven Algorithm, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2156, https://doi.org/10.5194/egusphere-egu25-2156, 2025.

EGU25-2242 | Posters on site | GI2.4

A Conditional Neural Operator Approach for Resolution-Flexible and Parameter-Controlled Gravity Forward Modelling 

Ruiyuan Kang, Meixia Geng, Qingjie Yang, and Felix Vega

We present a novel approach to gravity forward modeling using conditional neural operators that establishes a forward generative model from the basin models and hyperparameters (reference basement depth, etc.) to gravity anomaly. Our methodology introduces an innovative adaptive embedding mechanism where scalar hyperparameters are first embedded into a 32-dimensional space and then adaptively expanded to match the dimensions of the basin depth model, enabling effective fusion with basin depth model data. Subsequently, Fourier Convolution Layers are employed to transform the fused data into gravity anomalies. The model demonstrates superior performance compared to existing convolutional neural networks on the test dataset, showcasing improved accuracy in capturing complex geological structures and their gravity responses. A key advantage of our architectural design is that it not only preserves the super-resolution capability of conventional neural operators but also enables controlled generation through different hyperparameters. This dual capability allows for both resolution-flexible modeling and parameter-controlled generation, while training on low-resolution data and producing high-resolution outputs, significantly reducing training data requirements and computational costs. The model's adaptive architecture effectively bridges the resolution gap between training and application scenarios, offering a practical solution for real-world geological surveys. Our results suggest that this approach could substantially improve the accessibility and applicability of gravity forward modeling in various geological settings, particularly in regions with limited high-resolution training data.

How to cite: Kang, R., Geng, M., Yang, Q., and Vega, F.: A Conditional Neural Operator Approach for Resolution-Flexible and Parameter-Controlled Gravity Forward Modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2242, https://doi.org/10.5194/egusphere-egu25-2242, 2025.

EGU25-2478 | Orals | GI2.4

International standards for responsible AI in disaster management 

Monique Kuglitsch and Elena Xoplaki

The combination of big data and AI/ML technologies shows tremendous promise within the domain of disaster management. So that benefits of AI/ML can be realized, and risks can be adverted, internationally agreed upon standards are an important mechanism. These can provide guidance on how to apply (and develop policy around) data collection and preprocessing, model training and evaluation, and operational implementation. In conjunction, they can cultivate interoperability and harmonization of AI-based systems. At the United Nations, the Global Initiative on Resilience to Natural Hazards through AI Solutions brings together experts from different disciplines (geosciences, disaster risk management, computer sciences) and sectors (government, research, NGO) to analyze use cases and lay the groundwork for such standards. Through proof-of-concept projects (e.g., HEU-funded MedEWSa), these standards can be further refined. Finally, through education and capacity building activities, the Global Initiative can help to democratize the responsible use of AI for this domain.

How to cite: Kuglitsch, M. and Xoplaki, E.: International standards for responsible AI in disaster management, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2478, https://doi.org/10.5194/egusphere-egu25-2478, 2025.

EGU25-4298 | ECS | Posters on site | GI2.4

Advances in the identification of geological discontinuities in boreholes with deep learning 

Rushan Wang, Martin Ziegler, Michele Volpi, and Andrea Manconi

Geological discontinuities significantly influence rock mass behaviour. Understanding the origin, setting, and properties of discontinuities is of major relevance, especially in boreholes. Traditionally, manual interpretation of borehole logs is done by geologists, a process that is time-consuming, costly, and subject to variability based on the interpreter's expertise. Recent advancements in artificial intelligence have made it feasible to use machine learning models and automatically detect and differentiate various features in digital images. In this study, we employ a state-of-the-art semantic segmentation model to tackle domain-specific challenges, enabling the identification of discontinuity types (e.g., natural faults, fault zones) and rock mass behaviour features (e.g., breakouts, induced cracks). We applied the SegFormer semantic segmentation model, which integrates a hierarchically structured transformer encoder with a multilayer perceptron (MLP). The borehole data used in this study was collected from the Mont Terri underground rock laboratory. Specifically, we labelled several high-resolution optical logs from one borehole and divided the dataset into training and testing subsets. The borehole considered is an experimental borehole designed to investigate the spatial and temporal evolution of damage around an underground opening in faulted clay shale. Our strategy achieved robust and accurate segmentation results on borehole images. Following segmentation, post-processing techniques were employed to extract critical information such as the total length of induced cracks and the total area of breakouts, as well as their locations and frequencies. The experimental results demonstrate high performance, with the pixel accuracy of 96 % in under three minutes for a 10-meter borehole. Our study lays the groundwork for future research by introducing a powerful tool for extracting geological structures and demonstrating the potential of AI models in geological analysis. By reducing processing time and increasing consistency in the identification, mapping, and classification of geological features, our approach can reveal spatial and temporal patterns associated with the evolution of rock masses.

How to cite: Wang, R., Ziegler, M., Volpi, M., and Manconi, A.: Advances in the identification of geological discontinuities in boreholes with deep learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4298, https://doi.org/10.5194/egusphere-egu25-4298, 2025.

EGU25-4404 | ECS | Orals | GI2.4

AI-Enhanced Meteorological Data Retrieval Systems for Improved Forecast Operations 

Byeongyeon Kim, Hayan Shin, Areum Cho, Junsang Park, Hyesook Lee, ChaeHun Park, Jinkyung Joe, Jaegul Choo, and Minjoon Seo

Meteorological data are vast and complex, and their rapid and accurate retrieval is essential for forecasting operations. However, traditional systems have struggled with limited search accuracy and inefficient processing speeds, hindering effective forecast support. To address these challenges, this study developed an AI-based system capable of performing speech recognition, URL search, extreme value detection, and local forecast error analysis. In speech recognition, the Whisper-large model achieved a character error rate (CER) of 3.19%, with GPU memory usage reduced by 15.7% and inference time by 38.18%, enabling real-time processing and scalability in multi-GPU environments. The URL search systems translated natural language inputs into SQL queries and URLs, achieving a Mean Reciprocal Rank (MRR) of 0.92, thereby enhancing data retrieval precision. The extreme value detection systems utilized GPT-4-based template augmentation to expand training data by approximately 111%, significantly improving detection performance and search accuracy. For local forecast error analysis, a prototype chatbot was implemented using prompt engineering and a Text-to-SQL model, allowing for the automated identification of inconsistencies in local forecasts and streamlining the analysis process. These systems have substantially enhanced operational workflows across meteorological tasks, facilitating rapid data retrieval through voice commands, precise responses to complex queries, and real-time analytical support. Future research will focus on further refining these technologies to tackle a wider range of meteorological challenges and integrate them into global forecasting systems for enhanced accuracy and reliability.

How to cite: Kim, B., Shin, H., Cho, A., Park, J., Lee, H., Park, C., Joe, J., Choo, J., and Seo, M.: AI-Enhanced Meteorological Data Retrieval Systems for Improved Forecast Operations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4404, https://doi.org/10.5194/egusphere-egu25-4404, 2025.

EGU25-4699 | ECS | Orals | GI2.4

S-wave velocity prediction of shale reservoirs based on explainable physically-data driven model 

Zhijun Li, Shaogui Deng, and Yuzhen Hong

The shear wave (S-wave) velocity is a key basis for shale reservoir development, particularly for fracability evaluation. Additionally, S-wave velocity also plays a significant role in prestack seismic inversion and amplitude versus offset (AVO) analysis. However, the actual logging data often lack S-wave velocity data, so it is of significant importance for S-wave velocity prediction. We propose a rapid and precise prediction method for the S-wave velocity in shale reservoirs based on class activation maps (CAM) model combined with physically constrained two-dimensional Convolutional Neural Network (2D-CNN). High sensitivity curves related to S-wave velocity are selected as the foundation. Meanwhile, based on the petrophysical theory of pore medium, the petrophysical model of complex multi-mineral components is established. The dispersion effect is reduced to a certain extent and the results are used to constrain the model. The Adam optimization algorithm is used to construct a 2D-CNN model under the constraint of petrophysical model. The CAM is obtained by replacing the global average pooling (GAP) layer with a fully connected layer, which in turn leads to interpretable results. Then, the model is applied to wells A, B1, and B2 in the southern Songliao Basin. Afterwards, comparisons are made with unconstrained model and petrophysical model. The results show that the correlation coefficients and relative errors in the three test wells are 0.96 and 2.14%, 0.97 and 2.35%, and 0.97 and 2.9%, respectively. The higher prediction accuracy and generalization ability of the new method is confirmed. Finally, we present the defined C-factor as a means of evaluating the extent of concern regarding CAMs in regression problems. The C-factor confirms that the focus of 2D-CNN can be significantly enhanced by incorporating the petrophysical model, thereby imposing physical constraints on the 2D-CNN. In addition, we establish the SHAP model to assist in proving the importance of constraints.

Keywords: S-wave velocity prediction; Physically constrained 2D-CNN; Petrophysical model; Class activation mapping technique; Explainable results

How to cite: Li, Z., Deng, S., and Hong, Y.: S-wave velocity prediction of shale reservoirs based on explainable physically-data driven model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4699, https://doi.org/10.5194/egusphere-egu25-4699, 2025.

EGU25-7000 | ECS | Posters on site | GI2.4

Multivariate generative modelling of subsurface properties with diffusion models  

Roberto Miele and Niklas Linde

Accurate multivariate parametrization of subsurface properties is essential for subsurface characterization and inversion tasks. Deep generative models, such as variational autoencoders (VAEs) and generative adversarial networks (GANs), are known to efficiently parametrize complex facies patterns. Nonetheless, the inherent complexity of multivariate modeling poses significant limitations to their applicability when considering multiple subsurface properties simultaneously. Presently, diffusion models (DM) offer state-of-the-art performance and outperform GANs and VAEs in several tasks of image generation. In addition, training is much more stable compared to the training of GANs. In this work, we consider score-based DMs in multivariate geological modeling, specifically for the parametrization of categorical (facies) and continuous (acoustic impedance – I­P) distributions, focusing on a synthetic scenario of sand channel bodies in a shale background. We benchmark modeling performance against results obtained by GAN and VAE networks previously proposed in literature for multivariate modeling. As for the GAN and VAE models, the DM was trained with a training dataset of 3000 samples, consisting of facies realizations and co-located I­P geostatistical realizations. Overall, the trained DM shows significant improvements in modeling accuracy, for all evaluation metrics considered in this study, except for the sand-to-shale ratio, where the values are comparable to those of the GAN and VAE. In particular, the DM is 26% more accurate at reproducing the average (nonstationary) facies distribution and up to 90% more accurate at reproducing the IP marginal distributions for both sand and shale classes. Higher accuracy is also found in the reproduction of the facies-to-I­P joint distribution, whereas the spatial I­P distributions generated by the DM honour the two-point statistics of the training samples. The iterative generative process in DMs generally makes these networks more computationally demanding than VAEs and GANs. However, we demonstrate that with appropriate network design and training parametrization, the DM can generate realizations with significantly fewer sampling iterations while maintaining accuracy comparable to these benchmarking networks. Finally, since the proposed DM parametrizes the joint prior probability density function with a Gaussian latent space, it is straightforward to perform inversion. In addition to improved modeling accuracy, the mapping between the latent and image representations preserves a better topology than that of GANs, overcoming the well-known limitation of the latter for inference tasks, particularly for gradient-based inversion.

How to cite: Miele, R. and Linde, N.: Multivariate generative modelling of subsurface properties with diffusion models , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7000, https://doi.org/10.5194/egusphere-egu25-7000, 2025.

EGU25-9590 | Posters on site | GI2.4

Dynamic Time Warping algorithm: A geoscience aware AI for automatic interpretation in lithostratigraphy? Insights from an application to the Gulf of Corinth (Greece) 

Alina-Berenice Christ, Zahraa Hamieh, John Armitage, Renaud Divies, Sébastien Rohais, Luca Mattioni, and Antoine Bouziat

Stratigraphic correlation of well log data is a fundamental step in geosciences. It involves correlating stratigraphic units across multiple wells to build a comprehensive understanding of subsurface geology. Currently, stratigraphic correlation is predominantly performed “manually” by geoscientists. The process is labor-intensive and time-consuming, and interpretations may vary among interpreters due to differences in expertise, experience, and perspective.

Recent advancements in the application of the Dynamic Time Warping (DTW) algorithm have demonstrated its potential to automate and enhance the stratigraphic correlation of well logs. DTW can generate multiple correlation scenarios highlighting different interpretations of subsurface continuity. Thus, the aim of this work is to explore the potential of DTW as a supporting tool in the standard workflows of geoscientists and test it on well log data from IODP Expedition 381 from the Gulf of Corinth. We automatically correlate lithostratigraphic subunits within a 700 m thick stratigraphic unit across two wells, using Natural Gamma Ray (NGR) and Magnetic Susceptibility (MAGS) logs. We selected this dataset because it illustrates the evolution of geological interpretations over time. Between the first version of the IODP data interpretations and a second version published a few years later, significant differences in interpretation were proposed. These differences highlight the critical role of geological expertise in refining subsurface data interpretations and correlations.

The automatic correlations interpreted by DTW showed a minimal average absolute difference with the most recent and updated published correlation, making the human and the machine correlation almost identical. By applying DTW to this dataset, we demonstrate it would have been possible to identify discrepancies and challenges in the interpretations of subunits at the initial stages after data acquisition. This approach could have flagged potential issues even before the IODP data were made available on the public site. Such early identification highlights the potential of DTW as a valuable tool for providing immediate feedback and guiding more accurate stratigraphic interpretations faster.

While DTW significantly reduces the time required for the correlation phase, the time investment needed for data formatting upstream should not be underestimated. Future work on larger datasets will be crucial to better quantify and validate the overall time savings provided by DTW, as well as to optimize the preparatory steps to ensure efficiency in broader applications.

In conclusion, we show that DTW can offer innovative approaches to enhance geological investigations and speed up interpretations. More generally, we consider this work illustrates how data science methods can be leveraged to assist geologists in routine tasks, with our Corinth case study highlighting both the promises and current limitations of digital transformation in well correlations.  

How to cite: Christ, A.-B., Hamieh, Z., Armitage, J., Divies, R., Rohais, S., Mattioni, L., and Bouziat, A.: Dynamic Time Warping algorithm: A geoscience aware AI for automatic interpretation in lithostratigraphy? Insights from an application to the Gulf of Corinth (Greece), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9590, https://doi.org/10.5194/egusphere-egu25-9590, 2025.

EGU25-9671 | ECS | Orals | GI2.4

Kalpa: Empowering Artificial Intelligence-Driven Geospatial Analysis for Multidisciplinary Applications 

Sudhir Sukhbir, Satyam Pratap Singh, Utpal Singh, Mohit Kumar, and Tushar Goyal

In the age of big data, artificial intelligence (AI) is transforming Earth sciences by enabling efficient analysis and visualisation of complex datasets and fostering innovative approaches to solve age-old geoscientific challenges. Kalpa, a Python-based free and cross platform software, represents a pioneering step in this direction. Built with versatility at its core, Kalpa seamlessly integrates AI and machine learning workflows into geoscience applications, offering  customization through its Python plugin architecture. What sets Kalpa apart is its ease of use, even for non-experts. Its intuitive interface lowers the learning curve, enabling a broader audience—including researchers, professionals, and enthusiasts—to leverage advanced geospatial and AI tools without requiring extensive technical expertise.

Kalpa's capabilities span advanced 3D visualization, geospatial data processing, and machine learning model development. It supports global and regional raster and vector dataset visualisation and processing, allowing for interactive analysis in both geographic and cartesian coordinates. With tools to process satellite imagery, geological and geophysical data, uncrewed aerial vehicle (UAV) data, and digital geological maps, Kalpa caters to a wide range of applications, from mineral exploration to natural hazard forecasting. Its machine learning integration supports supervised and unsupervised algorithms for applications such as lithological mapping, mineral prospectivity mapping, land cover and land usage studies, agricultural productivity mapping and natural disaster management. In this study, we demonstrate Kalpa’s transformative potential through three case studies:

  • Lithological Mapping in Ladakh, India: Utilizing LANDSAT and SRTM data, we produced accurate lithological maps for this geologically complex region.
  • Copper Prospectivity Mapping in Northwest India: Combining remote sensing, geophysical, and geological data, Kalpa predicted copper mineralization zones, with all known deposits falling within areas of predicted probabilities exceeding 0.70.
  • Landslide Susceptibility Mapping in Uttarakhand, India: Using remote sensing datasets, Kalpa identified high-risk landslide zones, supporting disaster management efforts.

Kalpa’s user-friendly interface, robust machine learning integration, and publication-ready export capabilities position it as a powerful tool for advancing geoscience research and practical applications. By bridging the gap between domain expertise and cutting-edge AI methodologies, Kalpa empowers Earth scientists, environmental researchers, and GIS professionals to analyze, model, and predict with unprecedented efficiency and precision. This software marks a new frontier in the application of AI to Earth sciences, enabling multidisciplinary research and fostering innovative solutions to pressing geoscientific challenges.

How to cite: Sukhbir, S., Singh, S. P., Singh, U., Kumar, M., and Goyal, T.: Kalpa: Empowering Artificial Intelligence-Driven Geospatial Analysis for Multidisciplinary Applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9671, https://doi.org/10.5194/egusphere-egu25-9671, 2025.

EGU25-9968 | ECS | Posters on site | GI2.4

Advancing Landscape Archaeology with AI-driven insights from Airborne Laser Scanning data 

Nejc Coz, Žiga Kokalj, Susan Curran, Anthony Corns, Dragi Kocev, Ana Kostovska, Stephen Davis, and John O'Keeffe

Artificial intelligence (AI) is transforming landscape archaeology by enabling the automated analysis of high-resolution datasets, such as airborne laser scanning (ALS). The Automatic Detection of Archaeological Features (ADAF) tool is an example of the potential of AI to streamline the identification of subtle surface features and demonstrate their value in uncovering and understanding archaeological landscapes. By improving the detection of archaeological sites, the ADAF plays a crucial role in the research, management and preservation of cultural heritage.

ADAF uses advanced AI models, including convolutional neural networks (CNNs) for semantic segmentation and object detection, to detect features in ALS datasets. The tool has been trained on a large archive of ALS data from Ireland and processes visualised inputs to detect patterns indicative of archaeological structures. The workflow integrates pre-processing with the Relief Visualisation Toolbox, inference with trained AI models and post-processing to refine the results to ensure reliable outputs with minimal false positives.

Designed with accessibility in mind, ADAF features an intuitive user interface that removes the barriers traditionally associated with AI-driven analyses. Users can process ALS data and export GIS-compatible results without the need for specialised knowledge, making the tool suitable for a wide audience. This approach democratises the use of AI in landscape archaeology and extends its utility to professionals and researchers in the field.

Tests with Irish ALS datasets have shown that ADAF is able to detect both known and previously unrecognised archaeological features in the landscape, while enhancing the spatial accuracy of identified sites. By automating complex data analysis, ADAF underlines the efficiency, precision and scalability of AI in landscape archaeology. In addition, the tool contributes to the preservation of cultural heritage by identifying sites that would otherwise remain undiscovered and enabling their preservation and integration into cultural heritage management strategies.

ADAF represents a significant advance in the application of AI in landscape archaeology, providing a powerful and accessible solution for surface feature recognition. Its development underlines the transformative potential of AI to revolutionise the study and interpretation of archaeological landscapes.

How to cite: Coz, N., Kokalj, Ž., Curran, S., Corns, A., Kocev, D., Kostovska, A., Davis, S., and O'Keeffe, J.: Advancing Landscape Archaeology with AI-driven insights from Airborne Laser Scanning data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9968, https://doi.org/10.5194/egusphere-egu25-9968, 2025.

Borehole images (BHI) are crucial for resource exploration, providing detailed fracture analysis at millimeter-scale resolution. However, their interpretation is typically carried out manually, a process that is time-consuming, costly, and subject to significant uncertainty due to interpreter bias and variability. Current state-of-the-art AI methods for automated or semi-automated fracture analysis of BHI often rely on field data for training, using manual interpretations as labels. This approach inherently embeds both aleatoric (data-related) and epistemic (manual) uncertainties, which may undermine the reliability and adaptability of these methods. This study proposes an alternative, synthetic data-driven approach to train a set of two deep neural networks (DNNs) connected in sequence. These DNNs are designed to replicate the primary cognitive tasks involved in manual interpretation: the segmentation of the BHI to identify potential edge zones and the tracing of sinusoids over these edges to approximate their best-fitting 2D representation. By utilizing synthetic data, we are able to systematically assess the sensitivity of both networks and explore various training strategies, including curriculum learning (CL) and self-attention mechanisms. Our proposed solution is designed for post-hoc human-machine collaboration, where the model supports but does not replace human expertise. This framework enables the possibility of a multi-level uncertainty assessment—at the human, machine, and human-machine interface levels—opening the door to new ways of understanding and quantifying the sources of uncertainty in BHI analysis. Additionally, the synthetic data-driven approach ensures the generalizability and scalability of the method, as demonstrated by its successful application to low-resolution logging-while-drilling (LWD) and high-resolution fullbore formation microimager (FMI) datasets from multiple global locations. By combining advanced AI techniques with geoscientific knowledge, this study outlines a potential pathway toward more robust, ethical, and sustainable fracture analysis workflows. Beyond the traditional benefits of reduced cost and time, the approach may provide a scientifically grounded framework for exploring the benefits of human-machine collaboration and uncertainty quantification in geoscience practices. If adopted, this framework could significantly advance the field of BHI analysis, offering new tools for resource exploration in hydrocarbon and geothermal applications.

How to cite: Molossi, A., Roncoroni, G., and Pipan, M.: NeuroFit: a robust and scalable synthetic data-driven deep learning solution for automated borehole image analysis at LWD and wireline resolution, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10472, https://doi.org/10.5194/egusphere-egu25-10472, 2025.

EGU25-11754 | ECS | Orals | GI2.4

Exploring Pretraining Possibilities of Crop Classifiaction Models Using Large-Scale Sentinel-1 Datasets 

Mátyás Richter-Cserey, Máté Simon, Gabriel Magyar-Santen, Vivien Pacskó, and Dániel Kristóf

Since 2014, ESA Sentinel missions have been producing an ever-growing amount of data for Earth Observation. This creates the opportunity to monitor changes in high temporal and spatial resolution, however, interpreting this huge quantity of data is challenging. In recent years, the rapid advancement and widespread adoption of applied Artificial Intelligence (AI) methods made it feasible to create deep learning models for specific Earth Observation applications. Combining Sentinel datasets with the appropriate amount of ground truth, robust pre-trained models can be created and applied to produce good-quality thematic maps for different years and large areas. Due to responsibilities related to the European Union’s Common Agriculture Policy (CAP) and the motivation for regional yield estimation, crop classification is one of the most frequently studied remote sensing problems these days. Several papers investigate the possible methods to construct robust and generally functioning models to map the spatial distribution of crops as accurately as possible.

In this study, we present the development of a modular, pre-trained deep learning model designed specifically for crop type mapping. The model is tailored to classify the most prevalent crops in Hungary, including winter and autumn cereals, corn, sunflower, alfalfa, rapeseed, grasslands, and other significant types. For pre-training, we leverage country-wide Sentinel-1 Synthetic Aperture Radar (SAR) data such as Sigma Naught or polarimetric descriptors from H-A-alpha decomposition, collected during the 2021–2024 time period. This dataset comprises annual time series of Sentinel-1 pixels at a spatial resolution of 20 meters. Our approach builds upon prior findings that Sentinel-1-based crop type classification performs comparably to methods using Sentinel-2 optical data. However, Sentinel-1 has the added advantage of producing consistent and regular time series, as it is unaffected by atmospheric conditions such as cloud cover.

The proposed model employs a hybrid methodology integrating self-supervised and fully supervised learning paradigms. This modular architecture allows for seamless integration of task-specific classifiers, which can be fine-tuned using supervised learning to address both current and future classification requirements effectively. The fully supervised component is supported by an extensive ground truth dataset covering over 60% of Hungary’s total land area. This proprietary dataset is derived from the national agricultural subsidy database, providing detailed and accurate annotations. The abundance and quality of labeled data enable the construction of robust, highly generalizable models, ensuring reliable performance across diverse classification tasks. This methodology offers great potential to advance national-scale operational tasks, such as early land cover prediction and annual crop type mapping.

How to cite: Richter-Cserey, M., Simon, M., Magyar-Santen, G., Pacskó, V., and Kristóf, D.: Exploring Pretraining Possibilities of Crop Classifiaction Models Using Large-Scale Sentinel-1 Datasets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11754, https://doi.org/10.5194/egusphere-egu25-11754, 2025.

EGU25-12065 | ECS | Orals | GI2.4

Calibration of the Hypoplastic Clay model with a deep neutral network 

Phuong Do and Tomas Kadlicek

Advanced constitutive models, here represented by the hypoplastic clay model, are powerful tools which provide engineers with reliable responses in various practical applications. However, the model calibration is not an easy task. Calibration of these models can be addressed with several approaches, which are generally distinguished as stochastic or deterministic approaches. In general, these approaches extract information from the experimental data and the subsequent optimisation process finds the best combination of parameters to fit the desired constraints. . The deterministic approach was integrated and combined in development of the online automated calibration tool ExCalibre. This paper presents a Machine Learning approach for automated calibration of the Hypoplastic Clay model. By using pairs of input experimental data and calibrated results performed by ExCalibre as training data, a Deep Neural Networks (DNNs) model is constructed to recognise how the experimental data can be used to derive the asymptotic state parameters such as the slope and the interception of the Normal Compression Line (NCL), or the critical friction angle, and the optimised stiffness parameters. The training and testing data comprise of In-house protocols and User-upload data over 3 years of launching the ExCalibre, and synthetic data with small distortion to prevent overfitting. Finally, investigations on how the DNNs model recognises the asymptotic patterns, as well as its calibration results will be presented.

How to cite: Do, P. and Kadlicek, T.: Calibration of the Hypoplastic Clay model with a deep neutral network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12065, https://doi.org/10.5194/egusphere-egu25-12065, 2025.

EGU25-12242 | Posters on site | GI2.4

Automated Particle Size Distribution Estimation of Rock Avalanches using Deep Learning 

Ruoshen Lin, Michel Jaboyedoff, Marc-Henri Derron, and Tianxin Lu

Accurate estimation of Particle Size Distribution (PSD) in rock avalanche deposits is essential for understanding the fragmentation processes and spatial distribution characteristics during mass movement. However, traditional methods, such as physical sieving or visual field estimation, are time-consuming, labor-intensive, and impractical for large-scale field measurements. To address these limitations, this study presents an automated PSD estimation framework that combines UAV imagery and deep learning-based segmentation. A synthetic dataset was used to train the segmentation model, improving its robustness across different scenarios. Image resolution adjustments were applied to improve detection accuracy for small and overlapping particles. Additionally, Fourier analysis was utilized to reconstruct smooth and continuous particle contours, to effectively handle overlapping particles. The reconstructed 2D outlines were further used to estimate 3D particle volumes through the shape-volume model based on laboratory and literature data. Projection correction was applied to mitigate image distortions to ensure precise volume predictions. The proposed approach overcomes the limitations of traditional methods dealing with complex particle distributions in real field environments. The results demonstrate the effectiveness of the proposed method for large-scale particle detection and volume estimation, providing new insights into rock avalanche fragmentation dynamics.

Keywords: Rock avalanche; Particle size distribution (PSD); deep learning; UAV Imagery

How to cite: Lin, R., Jaboyedoff, M., Derron, M.-H., and Lu, T.: Automated Particle Size Distribution Estimation of Rock Avalanches using Deep Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12242, https://doi.org/10.5194/egusphere-egu25-12242, 2025.

EGU25-12675 | ECS | Orals | GI2.4

Automatic Detection of Cimiciato Defect in Hazelnuts Using Deep Learning and X-ray Radiography 

Antonio Gaetano Napolitano, Giacomo Mele, Laura Gargiulo, Matteo Giaccone, and Andrea Vitale

Hazelnuts are a significant crop, with global production exceeding 1.25 million tons by 2023 (INC, 2023). Quality is threatened by biotic agents, including insects causing the cimiciato defect. This defect, from insect bites during fruit growth, results in off-flavor, tissue alterations, and lipid oxidation (De Benedetta et al., 2023). Damage can be external or internal (hidden cimiciato). Industrial quality standards often exceed official regulations, making effective selection crucial. Traditional visual inspection is time-consuming and subjective. Non-destructive methods like NIR and NMR have potential but limited applicability. Deep Learning (DL) has revolutionized image classification, proving effective in agriculture, including disease and pest management (Mohanty et al., 2016; Dhaka et al., 2021; Meena et al., 2023). This study explores Deep Learning (DL) for automated detection of the cimiciato defect in hazelnuts using X-ray radiographs. Cimiciato, caused by insect feeding, degrades hazelnut quality, requiring product selection. Traditional methods are time-consuming and subjective. We propose a Convolutional Neural Network (CNN) model trained on X-ray images to classify hazelnuts as healthy or infected. Results demonstrate the model's effectiveness, offering a non-destructive, automated quality control solution.
Radiographs were acquired using a cone-beam micro-tomograph. Each hazelnut was positioned on a rotating stage. A CNN model was used for classification. CNNs effectively extract features from images. Convolutional layers apply filters to identify features; pooling layers reduce data dimensionality; fully connected layers combine features for classification. The Inception-ResNet-V2 architecture was chosen, combining Inception modules and residual connections (Szegedy et al., 2017). The model was trained (128 image batch size, 0.001 learning rate, 30 epochs), comparing SGD, ADAM, and RMSP optimizers. Images were pre-processed: resizing, pixel normalization, and data augmentation. 
The test dataset evaluated the trained network. SGD, ADAM, and RMSP yielded similar results. Confusion matrices visualize performance. ADAM performed best, but all achieved good results, especially for cimiciato detection. 

Keywords: Cimiciato defect, Hazelnut, Deep Learning, X-ray radiography, CNN

How to cite: Napolitano, A. G., Mele, G., Gargiulo, L., Giaccone, M., and Vitale, A.: Automatic Detection of Cimiciato Defect in Hazelnuts Using Deep Learning and X-ray Radiography, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12675, https://doi.org/10.5194/egusphere-egu25-12675, 2025.

EGU25-13315 | Posters on site | GI2.4

Harnessing AI and Decentralized Networks for Next-Generation Geophysical Forecasting 

Gabriel Moraga, Steven Hristopoulos, and Noah Pearson Kramer

Artificial Intelligence (AI) is revolutionizing geosciences, aligning perfectly with the themes of session GI2.4 by enabling the analysis of complex, multidimensional datasets and delivering actionable insights at unprecedented scales. This study presents two innovative AI-driven frameworks addressing critical challenges in soil moisture prediction and geomagnetic disturbance forecasting. Both approaches leverage decentralized networks to achieve scalability, foster collaboration, and enhance model performance through continuous refinement by a distributed community of contributors.

For soil moisture prediction, our multi-stream base model integrates data from Sentinel-2 (high-resolution spectral imagery), SMAP L4 (volumetric water content), ERA5 (meteorological variables), and SRTM (elevation data). The model predicts surface and rootzone soil moisture with six-hour lead times, achieving RMSE values of 0.1087 m³/m³ and 0.1183 m³/m³, respectively, across diverse Köppen-Geiger climate zones. By utilizing a decentralized network, contributors perform inference on 100 km² global regions, generating predictions evaluated against SMAP data using Root Mean Square Error (RMSE) and R² metrics. This system ensures robust model performance while addressing the spatial and temporal gaps inherent in traditional observational networks. These advances have significant implications for agriculture, hydrology, and climate modeling, enabling better water resource management, crop planning, and drought mitigation strategies. 

In geomagnetic disturbance forecasting, our GeoMagModel leverages Prophet, a time-series forecasting library, to predict the Disturbance Storm Time (Dst) index, a key indicator of geomagnetic activity. The model achieves an RMSE of 6.37 for December 2024 datasets, effectively capturing both trend shifts and weekly seasonality. The decentralized community enhances predictive accuracy by dynamically integrating historical and real-time Dst data, which is validated by benchmark predictions of the Kyoto World Data Center’s hourly records. This approach provides near-real-time forecasts critical for safeguarding power grids, satellite systems, and other infrastructure vulnerable to space weather events.

By integrating machine learning with decentralized computing and state-of-the-art data sources, these frameworks offer scalable solutions to longstanding challenges in geophysical monitoring. The decentralized network not only improves scalability but also incentivizes the geoscience community to refine baseline models, fostering innovation and enabling systems to outpace state-of-the-art benchmarks. The implications of this work extend beyond immediate applications, paving the way for hybrid models that combine AI-driven predictions with physical process-based simulations. This fusion has the potential to improve understanding and resilience in critical domains such as water resource planning, disaster mitigation, and space weather forecasting. By addressing the limitations of traditional observation systems and delivering actionable insights at scale, these AI-driven frameworks represent a paradigm shift in how we approach and solve complex geoscientific problems.

How to cite: Moraga, G., Hristopoulos, S., and Pearson Kramer, N.: Harnessing AI and Decentralized Networks for Next-Generation Geophysical Forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13315, https://doi.org/10.5194/egusphere-egu25-13315, 2025.

EGU25-15949 | ECS | Posters on site | GI2.4

Advanced Super-Resolution Techniques for Optical Payloads in Earth Observation: Combining Traditional and Deep Learning Methods 

Camilla De Martino, Vincenzo Della Corte, Laura Inno, Fabio Cozzolino, Giacomo Ruggiero, Vania Da Deppo, Paola Zuppella, Lama Moualla, and Sara Venafra

Small satellite platforms are increasingly used for Earth observation due to their cost-effectiveness and flexibility. However, their limited payload size often results in reduced spatial resolution of captured images. In our work, we address this challenge by proposing an advanced multi-image super-resolution (MISR) approach tailored for small satellite applications.

It integrates:

  • Sub-pixel image registration and on curvelet transform-based interpolation to preserve high-frequency details while reducing artifacts;
  • A novel hybrid method called SP-MISR (Subpixel Multi-Image Super-Resolution), which leverages Convolutional Neural Networks (CNNs) for local detail analysis and Transformers for global spatial relationships.

Our experimental results demonstrate that this combined approach  significantly improves image sharpness, preserves fine details, and reduces artifacts, outperforming traditional super-resolution techniques. Moreover, SP-MISR exhibits robustness in processing noisy and distorted images, making it particularly suitable for the constrained imaging systems of small satellites.

Future developments will focus on improving computational efficiency, reducing interpolation errors, and extending the method to multi-spectral imaging and interplanetary missions, by exploring explore pure deep learning techniques.

This work highlights the potential of integrating traditional and deep learning methodologies to enhance image quality, thus expanding the scientific and operational capabilities of small satellite missions.

How to cite: De Martino, C., Della Corte, V., Inno, L., Cozzolino, F., Ruggiero, G., Da Deppo, V., Zuppella, P., Moualla, L., and Venafra, S.: Advanced Super-Resolution Techniques for Optical Payloads in Earth Observation: Combining Traditional and Deep Learning Methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15949, https://doi.org/10.5194/egusphere-egu25-15949, 2025.

Soil carbonates are critical players in the global carbon cycle and have a profound influence on soil health and agricultural productivity. Their quantification is also central to carbon sequestration efforts, where accurate measurement of soil carbonates can inform strategies for reducing atmospheric CO2. However, conventional methods of carbonate analysis in soil---while effective---are often slow, costly, and labor-intensive (1).

In this study, we introduce Shifted Excitation Raman Difference Spectroscopy (SERDS) as a rapid, non-destructive alternative, further enhanced by advanced preprocessing techniques and machine learning algorithms. Specifically, we employ Asymmetric Least Squares (ALS) for background correction, Standard Normal Variate (SNV) for normalization, and Savitzky–Golay filtering for smoothing. Unlike conventional Raman spectroscopy, SERDS effectively eliminates background fluorescence and reduces overlapping peaks, resulting in clearer spectral signatures (2)

We employed Partial Least Squares Regression (PLSR) and eXtreme Gradient Boosting (XGBoost) to predict the inorganic carbon content from the carbonate vibrational modes in conventional Raman and SERDS spectra, benchmarked against total inorganic carbon (TIC) measurements from coulometric titration. Our results show that switching to dual-laser SERDS substantially boosted model performance. For PLSR, the coefficient of determination (R2) improved from 0.8 to 0.88 (an increase of about 10.5%), and the root-mean-square error (RMSE) declined from 0.29 to 0.22 (26% decrease). The XGBoost model exhibited an even greater increase, with R2 increasing from 0.63 to 0.93 (approximately 49% improvement) and RMSE dropping from 0.39 to 0.16 (59% reduction).

Figure 1: Left: All SERDS data of soil samples showing the main carbonate peak; Right: XGBoost model prediction of soil inorganic carbon using SERDS data.

These findings underscore the potential of SERDS to replace conventional methods for carbonate quantification, offering reduced cost, faster analysis, and essentially no sample preparation. Furthermore, by providing highly accurate carbonate measurements, this methodology can be pivotal for carbon sequestration assessments and large-scale soil management practices, helping to advance both environmental sustainability and agricultural productivity.

References:

1) Barra I, Haefele SM, Sakrabani R, Kebede F. Soil spectroscopy with the use of chemometrics, machine learning and pre-processing techniques in soil diagnosis: Recent advances–A review. TrAC Trends in Analytical Chemistry. 2021 Feb 1;135:116166.

2) Orlando A, Franceschini F, Muscas C, Pidkova S, Bartoli M, Rovere M, Tagliaferro A. A comprehensive review on Raman spectroscopy applications. Chemosensors. 2021 Sep 13;9(9):262.

How to cite: Poursorkh, Z., Solomatova, N., and Grant, E.: Quantifying Soil Inorganic Matter: Integrating Shifted Excitation Raman Difference Spectroscopy (SERDS) with Machine Learning for Enhanced Analysis of Carbonates, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16705, https://doi.org/10.5194/egusphere-egu25-16705, 2025.

Seismic exploration heavily relies on the accurate processing of seismic data, as high-quality reconstructed data is essential for reliable imaging and interpretation. In recent years, data-driven approaches have shown great promise in seismic data processing. However, supervised learning methods require large amounts of labeled data, while generative models, such as GANs, often encounter issues like mode collapse and instability. On the other hand, generative diffusion models, leveraging principles from nonequilibrium thermodynamics and Markov processes, have emerged as powerful tools for capturing complex data distributions.

Despite these advantages, Denoising Diffusion Probabilistic Models (DDPM) purely generate data distributions from the latent space with the reliance on random noise, making it inadequate for seismic data reconstruction where the goal is to accurately recover missing traces. Thus, DDPM is  lacks interpretability in seismic data restoration, and may disrupt the structured patterns crucial for interpolating seismic signals. Furthermore, we view the reverse process that starts from noise as unnecessary and inefficient for reconstruction task.

To address these challenges, we propose a novel Conditional Residual Diffusion Model (CRDM) that enhances both certainty and interpretability by incorporating residual diffusion and conditional constraints derived from observed seismic data (Fig.1). This approach better aligns with the inherent structure of seismic signals, enabling more accurate and interpretable reconstruction. The model is grounded in DDPM, with mathematical derivations for loss functions, conditional probability distributions, and reverse inference steps, ensuring both theoretical rigor and practical applicability.

Additionally, Our CRDM utilizes a shallow U-Net architecture featuring one down-sampling and one up-sampling layer integrated with Multi-Head Self-Attention (MHSA), which significantly enhances the model's efficiency and effectiveness. Experimental results (Fig.2) demonstrate that CRDM outperforms DDPM, denoising convolutional neural network (DnCNN), and fast projection onto convex sets (FPOCS), achieving a 15.1% improvement in reconstruction SNR and reducing computation time by 139 times compared to DDPM. Notably, CRDM achieves optimal results in a few diffusion steps, whereas DDPM typically requires thousands of steps.

The innovative approach generates data through residuals for determinism, while guiding the processing with noise for diversity. This not only enhances the interpretability and efficiency of seismic data reconstruction, but also positions the model as a promising tool for advancing data-driven seismic processing through flexible coefficient adjustment. Therefore, we believe this model has great potential for broader applications in geophysical data analysis, offering significant value in accurately depicting complex geological structures and providing more effective guidance for petroleum exploration.

Fig.1 The framework of CRDM. The model consists of two stage: (a) the training stage with forward diffusion process; (b) the sampling stage for seismic data reconstruction.

Fig.2 Reconstruction results and residuals of the 1994 BP seismic data with 50% irregular missing traces. (a) Complete data, reconstruction using (b) FPOCS (SNR=10.5dB), (c) DnCNN (SNR=15.6dB), (d) DDPM(SNR=18.4dB), (e) CRDM(SNR=21.2dB), and (f) observed seismic data with 50% missing traces. (g-j) display the residuals corresponding to reconstructions (b-e), respectively. The red box highlights a zoomed-in region, which is shown in detail in (k-t).

 

How to cite: Gong, X. and chen, S.: Enhancing Seismic Data Reconstruction with a Conditionally Constrained Residual Diffusion Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16835, https://doi.org/10.5194/egusphere-egu25-16835, 2025.

Recent trends in climate change and global warming have amplified the occurrence of severe convective initiation (CI) and other extreme weather events, underscoring the importance of high-frequency remote sensing. Modern satellite constellations such as EUMETSAT, GOES, Himawari, and GK2A now offer global monitoring intervals of 10 minutes and regional updates as frequent as 1–2 minutes. However, these capabilities are not universally accessible—many developing countries lack in-orbit assets or historical high-frequency data archives.

This study presents a zero-shot video frame interpolation (VFI) approach to generate high-frequency (1–10 minute) satellite imagery from legacy or sparsely sampled observations. Leveraging a flexible Many-to-Many Splatting VFI model, our framework avoids domain-specific retraining while delivering reliable intermediate frames. We validate the method using overlapping data from the KMA GK2A (10-minute full-disk, 2-minute Asia-Pacific) and KMA COMS (3-hour full-disk, 15-minute Asia-Pacific) satellites over the period July 25, 2019, to March 31, 2020.

Our results indicate significant improvements in both PSNR and SSIM metrics, confirming the model’s efficacy in three critical applications:

  • Up-sampling Archived Geostationary Data

    • Enhancing the temporal resolution of older satellite imagery (e.g., COMS 30-minute or 3-hour intervals) to match or approximate modern satellite capabilities (e.g., GK2A 10-minute intervals). This harmonization facilitates unified climatology analyses spanning multiple generations of instruments.
  • Sensor-Error Correction and Gap Filling

    • Recovering missing or corrupted frames resulting from attitude adjustments, sensor calibrations, or malfunctions on geostationary satellites. Ensuring a continuous record provides more robust inputs to operational forecasting and climate assessments.
  • Delayed High-Frequency Observation Services

    • Enabling resource-constrained meteorological agencies to retrospectively produce and disseminate high-frequency satellite products (e.g., near 1-minute intervals) to improve nowcasting, risk assessment, and disaster preparedness.

Our preliminary findings show minimal computational overhead per inference step, making this cost-effective method feasible for near-real-time deployment and post-event analyses alike. By bridging temporal gaps in global satellite datasets, this technique supports advanced level-2 products such as cloud-tracking and convective-initiation alerts, thereby driving broader socioeconomic and scientific benefits in both developed and developing regions.

How to cite: Ryu, H. and Choi, Y.: Toward High-Frequency Satellite Observations in Data-Sparse Regions: A Zero-Shot Interpolation Framework for Missing and Historical Imagery, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17456, https://doi.org/10.5194/egusphere-egu25-17456, 2025.

EGU25-17957 | Posters on site | GI2.4

Fuzzy clustering of electrical and seismic data for the detection of geophysical targets 

Giorgio De Donno, Michele Cercato, Davide Melegari, Valeria Paoletti, Guido Penta de Peppo, and Ester Piegari

Tomographic methods, such as electrical resistivity tomography (ERT), induced polarization (IP) and seismic refraction tomography (SRT) are often effective for detecting geophysical targets in disparate real-world scenarios. However, a final reconstruction expressed only in terms of individual geophysical parameters (resistivity, chargeability, P-wave velocity) leaves room for ambiguity in complex sites exhibiting several transitions between layers or zones having different geophysical properties. In such cases, the sensitivity of the geophysical parameters for the various methods can differ significantly, so that a univocal interpretation based only on a visual comparison of the different models is often ineffective. To overcome these limits, in this work we present a machine learning-based quantitative approach for the detection of geophysical targets associated with both geological and anthropogenic scenarios. We integrate two-dimensional ERT, IP and SRT tomographic data with a soft clustering analysis by the Fuzzy C-Means (FCM) to obtain a final combined section, where each pixel is characterized by a cluster index and an associated membership value. The membership function of the Fuzzy C-Means is a good estimator of the accuracy of the subsurface reconstruction, as it ranges from 0 to 1, with 1 reflecting a high reliability of the clustering analysis. We apply this method to two case studies, related to the detection of leachate accumulation areas in a municipal solid waste landfill and to the bedrock characterization in a site prone to instability. In both cases, we detect the cluster associated with the geophysical targets of interest and our final sections are validated by a good agreement with the available direct information (boreholes and wells). The accuracy of the reconstruction is consistently high across most areas (membership values > 0.75), even though it is reduced in areas where the resolution of geophysical data is lower. Therefore, this approach may be a valuable automatic tool for optimizing the cost-effectiveness of projects where new constructions or remediation interventions have to be planned.

How to cite: De Donno, G., Cercato, M., Melegari, D., Paoletti, V., Penta de Peppo, G., and Piegari, E.: Fuzzy clustering of electrical and seismic data for the detection of geophysical targets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17957, https://doi.org/10.5194/egusphere-egu25-17957, 2025.

EGU25-18082 | ECS | Orals | GI2.4

Integrating FDEM data with K-Means clustering for improved archaeological site identification 

Angelica Capozzoli, Valeria Paoletti, Federico Cella, Mauro La Manna, and Ester Piegari

The Frequency Domain Electromagnetic (FDEM) method is a cost-effective geophysical technique that simultaneously studies the electrical and magnetic properties of a medium, providing data as in-phase and out-of-phase components of the electromagnetic field. Although FDEM yields valuable insights, its results can be complex to interpret, and the two EM field components are normally only visually inspected to support findings from other techniques. This study aims to enhance FDEM data interpretation using an unsupervised learning technique. The proposed approach seeks to automate and expedite the interpretative phase. By applying the K-Means clustering algorithm, we divided the FDEM data into several clusters based on specific intervals of the in-phase and quadrature components, resulting in integrated maps of EM components. Combining these maps with geological and archaeological insights helped identifying areas of potential archaeological interest. This method was applied to the Torre Galli archaeological site in Calabria, Italy, known for its significance in Iron Age studies.

Based on comparisons with the findings of earlier excavations and results from a magnetic survey, the proposed procedure shows promise in improving the efficiency and accuracy of the FDEM method in identifying areas of archaeological interest. This suggests that automating the interpretation process could lead to a better cost management and time optimization in geophysical and archaeological studies.

How to cite: Capozzoli, A., Paoletti, V., Cella, F., La Manna, M., and Piegari, E.: Integrating FDEM data with K-Means clustering for improved archaeological site identification, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18082, https://doi.org/10.5194/egusphere-egu25-18082, 2025.

Artificial Intelligence (AI) is revolutionizing the field of geomorphology, offering a robust tool for objective and quantitative analyses. This pioneering study proposes an innovative framework based on Machine Learning clustering techniques, capable of classifying drainage patterns into multiple morphological classes. This work follows up on a related study in which an attempt at classifying 156 terrestrial and extraterrestrial (Mars and Titan) river networks was made. Rivers’ outlines are intrinsically noisy, difficult to isolate from the background, and can be ambiguous for the human eye. The previous works have been focused on accurately classifying patterns, using the expertise of morphologists, thus introducing a weak link, the human eye, in the chain. This time, a reliable, automatic, and scalable methodology has been obtained, leveraging computers’ precision, objectivity, and computational power. The HydroRIVERS dataset, a publicly available data bank containing vector data, was utilized in this study. All HydroRIVERS data layers are provided in a geographic projection (latitude/longitude), referenced to the WGS84 datum. Each data layer includes an attribute table with information on the morphometric characteristics of each river reach. The input parameters for the clustering models included morphometric features such as LENGTH_KM, DIS_AV_CMS, ORD_STRA, ORD_CLAS, and ORD_FLOW.
During a preliminary experiment, a local convexity test was conducted to determine the optimal number of clusters (k) to identify the best metric values. This test made sure that the number of clusters with the highest evaluation metric was selected, varying in a closed numeric interval. Each cluster corresponds to a specific river class. Significant results were obtained with k = 6, k = 8, k = 10, and k = 12. Subsequently, the K-Means algorithm was applied, grouping the dataset into distinct clusters based on the morphometric parameters. The results were remarkable, with 10 being the best value for k. The results indicate that the clustering algorithm is able to optimally separate the dataset, producing a high inter-cluster distance and a low intra-cluster distance. The dataset points along the features, as highlighted by the three principal components obtained by performing PCA on the final five-dimensional clustering resulting vector space, are well grouped in relatively small clusters, far away from each other. The next step involves using the centroids obtained from the analysis of the large dataset as a reference for classifying the 155 rivers. In general, the centroids obtained from this kind of Learning could be of great value to the scientific community, establishing a new and innovative way of discerning between different classes of rivers without having to manually analyze and inspect images. This approach promises efficient and accurate classification of both terrestrial and extraterrestrial drainage patterns.

How to cite: D'Aniello, M. and Donadio, C.: A novel approach using Machine Learning to objectively classify terrestrial and extraterrestrial river networks, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19838, https://doi.org/10.5194/egusphere-egu25-19838, 2025.

EGU25-20509 | Orals | GI2.4 | Highlight

Making Sense of AI: The Important Role of Education and Communication 

Luis Azevedo Rodrigues

The big developments in Artificial Intelligence (AI) generated a mixture of fascination and apprehension, echoing historical responses to unknown phenomena. Like how medieval European societies interpreted certain natural events and instruments as magical, AI is currently perceived by many as a “black box,” blurring the lines between advanced technology and mystical force. This phenomenon fosters misconceptions and uncertainties about AI’s actual mechanisms, benefits, and risks. Consequently, it underscores the urgent need for science communicators and science museums to adopt an active role in enhancing the general public’s AI literacy and in debunking some of its enigmatic traits.

By drawing parallels with the Middle Ages—when objects such as mirrors and magnetite were often attributed supernatural capabilities—modern AI tools LLMs or image and video generators are frequently viewed as possessing a “magical” principle. The public’s limited grasp of how AI processes inputs and produces outputs further intensifies this impression. The lack of transparency (or “black box” effect) in deep learning algorithms, combined with the ambiguity of human language, has been shown to fuel both wonder and anxiety.

Science museums and communicators should have an active role by offering educational programs that demystify AI through different demographic and social activities as well as promoting the public debate. These initiatives could clarify AI’s underlying mathematical and computational principles, highlight practical examples of AI-driven applications, and examine ethical considerations surrounding its deployment. Public understanding of AI’s capabilities and limitations is crucial not only to temper undue fears but also to encourage informed engagement with emerging technologies.

How to cite: Azevedo Rodrigues, L.: Making Sense of AI: The Important Role of Education and Communication, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20509, https://doi.org/10.5194/egusphere-egu25-20509, 2025.

EGU25-1294 | Posters on site | ESSI2.13

A new sub-chunking strategy for fast netCDF-4 access in local, remote and cloud infrastructures.  

Flavien Gouillon, Cédric Penard, Xavier Delaunay, and Sylvain Herlédan

NetCDF (Network Common Data Form) is a self-describing, portable and platform-independent format for array-oriented scientific data which has become a community standard for sharing measurements and analysis results in the fields of oceanography, meteorology but also in the space domain.

The volume of scientific data is continuously increasing at a very fast rate. Object storage, a new paradigm that appeared with cloud infrastructures, can help with data storage and parallel access issues, but NetCDF may not be able to get the most out of this technology without some tweaks and fine tuning.

The availability of ample network bandwidth within cloud infrastructures allows for the utilization of large amounts of data. Processing data       where the data is located is preferable as it can result in substantial resource savings. But for some use cases downloading data from the cloud is required (e.g. processing also involving confidential data) and results still have to be fetched once processing tasks have been executed on the cloud.

Networks      exhibit significant variations in capacity and quality (ranging from fiber-optic and copper connections to satellite connections with poor reception in degraded conditions on boats, among other scenarios). Therefore, it is crucial for formats and software libraries to be specifically designed to optimize access to      data by minimizing the transfer to only what is strictly necessary.

In this context, a new approach has emerged in the form of a library that indexes the content of netCDF-4 datasets. This indexing enables the retrieval of sub-chunks, which are pieces of data smaller than a chunk, without the need to reformat the existing files. This approach targets access patterns such as time series in netCDF-4 datasets formatted with large chunks.

This report provides a performance assessment of netCDF-4 datasets for varied use cases. This assessment executes these use cases under various conditions, including POSIX and S3 local filesystems, as well as a simulated degraded network connection. The results of this assessment may provide guidance on the most suitable and most efficient library for reading netCDF data in different situations.

How to cite: Gouillon, F., Penard, C., Delaunay, X., and Herlédan, S.: A new sub-chunking strategy for fast netCDF-4 access in local, remote and cloud infrastructures. , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1294, https://doi.org/10.5194/egusphere-egu25-1294, 2025.

EGU25-4155 | Orals | ESSI2.13

How open software, data and platforms are transforming Earth observation data science 

Wolfgang Wagner, Matthias Schramm, Martin Schobben, Christoph Reimer, and Christian Briese

One of the most time-consuming and cumbersome tasks in Earth observation data science is finding, accessing and pre-processing geoscientific data generated by satellites, ground-based networks, and Earth system models. While the much increased availability of free and open Earth observation datasets has made this task easier in principle, scientific standards have evolved according to data availability, now emphasizing research that integrates multiple data sources, analyses longer time series, and covers larger study areas. As a result of this “rebound effect”, scientists and students may find themselves spending even more of their time on data handling and management than in the past. Fortunately, cloud platform services such as Google Earth Engine can save significant time and effort. However, until recently, there were no standardized methods for users to interact with these platforms, meaning that code written for one service could not easily be transferred to another (Schramm et al., 2021). This created a dilemma for many geoscientists: should they use proprietary cloud platforms to save time and resources at the risk of lock-in effects, or rely on publicly-funded collaborative scientific infrastructures, which require more effort for data handling? In this contribution, we argue that this dilemma is about to become obsolete thanks to rapid advancements in open source tools that allow building open, reproducible, and scalable workflows. These tools facilitate access to and integration of data from various platforms and data spaces, paving the way for the “Web of FAIR data and services” as envisioned by the European Open Science Cloud (Burgelman, 2021). We will illustrate this through distributed workflows that connect Austrian infrastructures with European platforms like the Copernicus Data Space Ecosystem and the DestinE Data Lake (Wagner et al., 2023). These workflows can be built using Pangeo-supported software libraries such as Dask, Jupyter, Xarray, or Zarr (Reimer et al., 2023). Beyond advancing scientific research, these workflows are also valuable assets for university education and training. For instance, at TU Wien, Jupyter notebooks are increasingly used in exercises involving Earth observation and climate data, and as templates for student projects and theses. Building on these educational resources, we are working on an Earth Observation Data Science Cookbook to be published on the Project Pythia website, a hub for education and training in the geoscientific Python community.

References

Burgelman (2021) Politics and Open Science: How the European Open Science Cloud Became Reality (the Untold Story). Data Intelligence 3, 5–19. https://doi.org/10.1162/dint_a_00069

Reimer et al. (2023) Multi-cloud processing with Dask: Demonstrating the capabilities of DestinE Data Lake (DEDL), Conference on Big Data from Space (BiDS’23), Vienna, Austria. https://doi.org/0.2760/46796

Schramm et al. (2021) The openEO API–Harmonising the Use of Earth Observation Cloud Services Using Virtual Data Cube Functionalities. Remote Sensing 13, 1125. https://doi.org/10.3390/rs13061125

Wagner et al. (2023) Federating scientific infrastructure and services for cross-domain applications of Earth observation and climate data, Conference on Big Data from Space (BiDS’23), Vienna, Austria. https://doi.org/10.34726/5309

How to cite: Wagner, W., Schramm, M., Schobben, M., Reimer, C., and Briese, C.: How open software, data and platforms are transforming Earth observation data science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4155, https://doi.org/10.5194/egusphere-egu25-4155, 2025.

EGU25-4277 | Posters on site | ESSI2.13

BEACON Binary Format (BBF) - Optimizing data storage and access to large data collections 

Tjerk Krijger, Peter Thijsse, Robin Kooyman, and Dick Schaap

As part of European projects, such as EOSC related Blue-Cloud2026, EOSC-FUTURE and FAIR-EASE, MARIS has developed and demonstrated a software system called BEACON with a unique indexing system that can, on the fly with high performance, extract data subsets based on the user’s request from millions of heterogeneous observational data files. The system returns one single harmonised file as output, regardless of whether the input contains many different data types or dimensions. 

Since in many cases the original data collections that are imported in a BEACON installment contain millions of files (e.g. Euro-Argo, SeaDataNet, ERA5, World Ocean Database), it is hard to achieve fast responses. Next to this, these large collections also require a large storage capacity. To mitigate these issues, we wanted to optimize the internal file format that is used within BEACON. With the aim of reducing the data storage size and speeding up the data transfer, while guaranteeing that the information of the original data files is maintained. As a result, the BEACON software has included a unique file format called the “BEACON Binary Format (BBF)” that meets these requirements. 

The BBF is a binary data format that allows for storing multi-dimensional data as apache arrow arrays with zero deserialization costs. This means that computers can read the data stored on disk, as if it were computer memory, significantly reducing computational access time by eliminating the cost for a computer to translate what’s on disk, to computer memory.

Together with making the entire data format “non-blocking”, which means that all computer cores can access the file at the same time and simultaneously use the jump table to read millions of datasets in parallel. This enables a level of performance which reaches speeds of multiple GB/s, making the hardware the bottleneck instead of the software.

Furthermore, the format takes a unique approach to compressing data by adjusting the way it compresses and decompresses on a per dataset level. This means that every dataset is compressed in a slightly different manner, making it much more effective in terms of size reduction and time to decompress the data which can get close to the effective memory speed of a computer.

It does this while retaining full data integrity. No data is ever lost within this format, nor is any data adjusted. If one were to import a NetCDF file into BBF, one could fully rebuild the original NetCDF file from the BBF file itself. In the presentation the added benefits of using the BBF will be highlighted by comparing and benchmarking it to traditional formats such as NetCDF, CSV, ASCII, etc.

In January 2025, BEACON 1.0.0 was made publicly available as an open-source software, allowing everyone to set-up their own BEACON node to enhance the access to their data, while at the same time being able to reduce the storage size of their entire data collection without losing any information. More technical details, example applications and general information on BEACON can be found on the website https://beacon.maris.nl/.

How to cite: Krijger, T., Thijsse, P., Kooyman, R., and Schaap, D.: BEACON Binary Format (BBF) - Optimizing data storage and access to large data collections, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4277, https://doi.org/10.5194/egusphere-egu25-4277, 2025.

EGU25-5977 | Orals | ESSI2.13

A comparative study of algorithms for lossy compression of 2-d meteorological gridded fields 

Uwe Ehret, Jieyu Chen, and Sebastian Lerch

Meteorological observations (e.g. from weather radar) and the output of meteorological models (e.g. from reanalyses or forecasts) are often stored and used in the form of time series of 2-d spatial gridded fields. With increasing spatial and temporal resolution of these products, and with the transition from providing single deterministic fields to providing ensembles, their size has dramatically increased, which makes use, transfer and archiving a challenge. Efficient compression of such fields - lossy or lossless - is required to solve this problem.

The goal of this work was therefore to apply several lossy compression algorithms for 2d spatial gridded meteorological fields, and to compare them in terms of compression rate and information loss compared to the original fields. We used five years of hourly observations of rainfall and 2m air temperature on a 250 x 400 km region over central Germany on a 1x1 km grid for our analysis.

In particular, we applied block averaging as a simple benchmark method, Principal Component Analysis, Autoencoder Neural Network (Hinton and Salakhutdinov, 2006) and the Ramer-Douglas-Peucker algorithm (Ramer, 1972; Douglas and Peucker, 1973) known from image compression. Each method was applied for various compression levels, expressed as the number of objects of the compressed representation, and then the (dis-)similarity of the original field and the fields reconstructed from the compressed fields was measured by Mean Absolute Error, Mean Square Error, and the Image Quality Index (Wang and Bovik, 2002). First results indicate that even for spatially heterogeneous fields like rainfall, very high compression can be achieved with small error.

 

References

Douglas, D., Peucker, T.: Algorithms for the reduction of the number of points required to represent a digitized line or its caricature. In: The Canadian Cartographer. Bd. 10, Nr. 2, 1973, ISSN 0008-3127, S. 112–122, 1973.

Hinton, G. E., & Salakhutdinov, R. R.: Reducing the dimensionality of data with neural networks. science, 313(5786), 504-507, 2006.

Ramer, U.: An iterative procedure for the polygonal approximation of plane curves, Computer Graphics and Image Processing, 1, 244-256, http://dx.doi.org/10.1016/S0146-664X(72)80017-0, 1972.

Zhou Wang, and A. C. Bovik: A universal image quality index, IEEE Signal Processing Letters, 9, 81-84, 10.1109/97.995823, 2002.

How to cite: Ehret, U., Chen, J., and Lerch, S.: A comparative study of algorithms for lossy compression of 2-d meteorological gridded fields, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5977, https://doi.org/10.5194/egusphere-egu25-5977, 2025.

EGU25-7371 | ECS | Orals | ESSI2.13

Evaluating Advanced Scientific Compressors on Climate Datasets 

Robert Underwood, Jinyang Liu, Kai Zhao, Sheng Di, and Franck Cappello

    As climate and weather scientists strive to increase accuracy and understanding of our world, models of weather and climate have increased in their resolution to square kilometers scale and become more complex increasing their demands for data storage. A recent study SCREAM run at 3.5km resolution produced nearly 4.5TB of data per simulated day, and the recent CMIP6 simulations produced nearly 28PB of data. At the same time, storage and power capacity at facilities conducting climate experiments are not increasing at the same rate as the volume of climate and weather datasets leading to a pressing challenge to reduce data volumes. While some in the weather and climate community have adopted lossless compression, these techniques frequently produce compression ratios on the order of 1.3$\times$, which are insufficient to alleviate storage constraints on facilities. Therefore, additional techniques, such as science-preserving lossy compression that can achieve higher compression ratios, are necessary to overcome these challenges.

    While data compression is an important topic for climate and weather applications, many of the current assessments of the effectiveness of climate and weather datasets do not consider the state of the art in compressor design and instead, asses scientific compressors that are 3-11 years old, substantially behind the state of the art. In this report: 

 

  •  We assess the current state of the art in advanced scientific lossy compressors against the state of the art in quality assessment criteria proposed for the ERA5 dataset to assess the current gaps between needed performance requirements and the capabilities of the current compressors.
  • We present new capabilities that allow us to build an automated, user-friendly, and extensible pipeline for quickly finding compressor configurations that maximize compression ratios while preserving scientific integrity of the data using codes developed as part of the NSF FZ project.
  • We demonstrate a number of capabilities that facilitate use within in the weather and climate community including NetCDF, HDF5, and GRIB file format support; support for innovation via Python, R, and Julia as well as low level languages such as C/C++; and the implementations of commonly used climate quality metrics including dSSIM, and the ability to extend to add new metrics in high-level languages
  • Utilizing this pipeline, We find that with advanced scientific compressors, it is possible to achieve a 6.4x improvement or more in compression ratio over previously evaluated compressors

How to cite: Underwood, R., Liu, J., Zhao, K., Di, S., and Cappello, F.: Evaluating Advanced Scientific Compressors on Climate Datasets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7371, https://doi.org/10.5194/egusphere-egu25-7371, 2025.

EGU25-11118 | Orals | ESSI2.13

Too Big to Handle? Hexagonizing LIDAR and Satellite Data in Geoscience Applications 

Bo Møller Stensgaard, Casper Bramm, Marie Katrine Traun, and Søren Lund Jensen

The exponential growth of LIDAR and satellite data in geoscience presents both opportunities and challenges for users. Traditional data handling methods often struggle with the sheer volume and complexity of these datasets, hindering easy accessibility, efficient analysis and decision-making processes. This presentation introduces the Scandinavian Highlands HEX-Responder platform and database structure, a cutting-edge solution that leverages the power of hexagonal discrete global grid system, Uber H3, and developed processes to revolutionize geospatial data management, fast responsive visualization and analysis.

We will showcase real-world applications, highlighting the platform's potential to accelerate scientific discovery and improve decision-making processes using satellite and remote sensing data.

The platform’s approach offers several advantages over conventional methods:

  • Efficient data organization and retrieval
  • Improved advanced spatial data analyses opportunities
  • Seamless integration of multi-scale and multi-dimensional data without losing information
  • Enhanced, responsive and fast visualisation capabilities

Our ELT (extract, load, transform) and subsequent visualisation procedure can be applied to any big raster data formats. First, the raw raster data is transformed into optimised parquet files through chunked reading and compression based on a low-resolution H3 hexagon cell index (hexagonization), enabling rapid data import to a column-oriented database management system for big data storage, processing and analytics. The H3 cell organisation is preserved in the database through partitioned fetching for visualisation on the platform. This method allows for horizontal scaling and accurate multi-resolution aggregation, preserving data integrity across scales and significantly overcomes typical computational memory limitations.

The platform's capabilities are exemplified by its approach to LIDAR and satellite emissivity data processing using the H3 grid. High-resolution LIDAR data is efficiently gridded and visualized to H3 resolution level 15 hexagons (0.9m2 hexagon cells). The gridding preserves all original pixel raster points while providing aggregated views for seamless zooming.

Another prime example of the capabilities is the handling of NASA’s ASTER Global Emissivity Data (100m resolution). Here, our pipeline transformed 2.1 terabytes of extracted raw CSV-data derived from NASA’s emissivity data into a compressed format based on the H3 index occupying only 593 gigabytes in the database.

This approach not only saves data storage space but also dramatically improves data accessibility and processing speed for the users, allowing users to work in a responsive environment with this massive dataset in ways previously not possible. Each hexagon represents an opportunity to store unlimited amount, types and categories of pre-processed data for more integrative analyses and data insight.

By hexagonizing LIDAR and satellite data, the HEX-Responder platform enables users to explore massive datasets with ease and efficiency in a responsive environment. The integrated procedures allow for detailed information maintenance and retrieval, paving the way for advanced predictive modelling in geoscience applications using earth observation data in a new way.  

How to cite: Stensgaard, B. M., Bramm, C., Traun, M. K., and Jensen, S. L.: Too Big to Handle? Hexagonizing LIDAR and Satellite Data in Geoscience Applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11118, https://doi.org/10.5194/egusphere-egu25-11118, 2025.

EGU25-12760 | ECS | Posters on site | ESSI2.13

Tree-Based Adaptive Data Reduction Techniques for Scientific Simulation Data 

Niklas Böing, Johannes Holke, Achim Basermann, Gregor Gassner, and Hendrik Fuchs

Large-scale Earth system model simulations produce huge amounts of data. Due to limited I/O bandwidth and available storage space this data often needs to be reduced before written to disk or stored permanently. Error-bounded lossy compression is an effective approach to tackle the trade-off between accuracy and storage space.

We are exploring and discussing lossless as well as error-bounded lossy compression based on tree-based adaptive mesh refinement/coarsening (AMR) techniques. Our lossy compression schemes allow for absolute and relative error bounds. The data reduction methods are closely linked to an underlying (adaptive) mesh which easily permits error regions of different error tolerances and criteria – in particular, we allow nested domains of varying error tolerances specified by the user. Moreover, some of the compressed data structures allow for an incremental decompression in the resolution of the data which may be favorable for transmission and visualization.

We implement these techniques as the open source tool cmc, which is based on the parallel AMR library t8code. The compression tool can be linked to and used by arbitrary simulation applications or executed as a post-processing step. We show different application results of the compression in comparison to current state-of-the-art compression techniques on several benchmark data sets.

How to cite: Böing, N., Holke, J., Basermann, A., Gassner, G., and Fuchs, H.: Tree-Based Adaptive Data Reduction Techniques for Scientific Simulation Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12760, https://doi.org/10.5194/egusphere-egu25-12760, 2025.

EGU25-13394 | ECS | Orals | ESSI2.13

Challenges and perspectives of climate data compression in times of kilometre-scale models and generative machine learning 

Milan Klöwer, Tim Reichelt, Juniper Tyree, Ayoub Fatihi, and Hauke Schulz

Climate data compression urgently needs new standards. The continuously growing exascale mountain of data requires compressors that are widely used and supported, essentially hiding the compression details from many users. With the advent of AI revolutionising scientific computing, we have to set the rules of this game. Minimizing information loss, maximising compression factors, at any resolution, grid and dataset size, for all variables, with chunks and random access, while preserving all statistics and derivatives, at a reasonable speed — are squaring the compression circle. Many promising compressors are hardly used as trust among domain scientists is hard to gain: The large spectrum of research questions and applications using climate data is very difficult to satisfy simultaneously.

Here, we illustrate the motivation behind the newly defined climate data compression benchmark ClimateBenchPress, designed as a quality check in all those dimensions of the problem. Any benchmark will inevitably undersample this space, but we define datasets from atmosphere, ocean, and land as well as evaluation metrics to pass. Results are presented as score cards, highlighting strengths and weaknesses for every compressor.

The bitwise real information content shows a systematic way in case no error bounds are known. In the case of the ERA5 reanalysis, errors are estimated and allow us to categorize many variables into linear, log and beta distributions with values bounded from zero, one or both sides, respectively. This allows us to define error thresholds arising from observation and model errors directly, providing another alternative to the still predominant subjective choices. Most error-bounded compressors come with parameters that can be automatically chosen following this analysis.

Also new data formats are on the horizon: Chunking and hierarchical data structures allow and force us to adapt compressors to spatially or length-scale dependent information densities. Extreme events, maybe counterintuitively, often increase the compressibility through higher uncertainties, but lie on the edge or outside of the training data for machine learned-compressors. This again increases the need for well-tested compressors. Benchmarks like ClimateBenchPress are required to encourage new standards for safe lossy climate data compression.

How to cite: Klöwer, M., Reichelt, T., Tyree, J., Fatihi, A., and Schulz, H.: Challenges and perspectives of climate data compression in times of kilometre-scale models and generative machine learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13394, https://doi.org/10.5194/egusphere-egu25-13394, 2025.

EGU25-13567 | Posters on site | ESSI2.13

Tables as a way to deal with a variety of data formats and APIs in data spaces 

Joan Masó, Marta Olivé, Alba Brobia, Nuria Julia, Nuria Cartell, and Uta Wehn

The Green Deal Data Space is born in the big data paradigm where there is a variety of data formats and data models that are exposed as files or web APIs. As a result, we need to default in simple data structure that is transversal enough to be able to represent most of the more specific data models, formats and API payloads. Many data models present a structure that can be represented as tables.

TAPIS stands for "Tables from APIS". It is a JavaScript code that uses a common data model that is an array of objects with a list of properties that can contain a simple or a complex value. In TAPIS offers a series of operations that use one or more arrays of objects as inputs and produce a new array of objects as an output. There are operations that create the arrays of objects from files or API queries (a.k.a. data import), others that manipulate the objects (e.g. merge two arrays in a single one) and some operations that generate visual representations of the common data structure including tabular, a map, a graph, etc.

TAPIS is limited by its own data model. While many of the data models can be mapped to the common data model, a multidimensional data cube or a data tree cannot be represented in a single table in an efficient way. In the context of the Green Deal Data Space, most of the sensor data, statistical data, geospatial feature based data and administrative data can be considered object based data and can be used in TAPIS. TAPIS is able to connect to Sensor Things API (the sensor protocol selected in AD4GD and CitiObs), S3 buckets (the internal cloud repository used in AD4GD), GeoNetwork (the geospatial metadata catalogue selected in AD4GD and more4nature), and the OGC API features and derivates (the modern web API interfaces standardized by the OGC) but other data inputs will be incorporated, such as Citizen Science data sources and other popular APIs used in the more4nature project. More analytical functionalities are going to be incorporated in the CitiObs project. As part of the AD4GD Green Deal Information Model, there is an operation to associate semantics to each column of a table by linking it to a URI that defines the concept in an external vocabulary (as well as units of measure if appropriate). In order to be compatible with the data space architecture recommended by the International Data Space Association, we are working on supporting the catalogue of the Eclipse Data Connector, and to be able to negotiate a digital contract as a previous step to request access to the relevant data offered in the data space. To do so, we are working on incorporating the data space protocol as part of the TAPIS operations for data import. TAPIS is available as open source at https://github.com/joanma747/TAPIS.

AD4GD, CitiObs and more4nature are Horizon Europe projects co-funded by the European Union, Switzerland and the United Kingdom.

How to cite: Masó, J., Olivé, M., Brobia, A., Julia, N., Cartell, N., and Wehn, U.: Tables as a way to deal with a variety of data formats and APIs in data spaces, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13567, https://doi.org/10.5194/egusphere-egu25-13567, 2025.

Early career scientists rarely have the resources to work with earth observation data at continental to global scale. This is caused by a combination of factors: large scale data analysis often involves teamwork, connecting data scientists, code developers, IT specialists, statisticians and geoscientists. Young researchers are rarely able to coordinate such a team. Meanwhile, all scientists can have relevant ideas or pose powerful research questions that merit investigation. Copernicus Data Space Ecosystem provides a public, free platform for large-scale processing of earth observation data. It combines instant access to all Sentinel satellite imagery with cloud-based processing in the form of API requests and a powerful browser-based viewing interface. This new approach is enabled by storing the data in a different way: uncompressed formats such as JPEG2000, COG or ZARR support subsetting and querying the image rasters without first unzipping the file, thereby allowing direct streaming of only the area and bands that the user requests. Additionally, this means that most calculations and visualization tasks can be carried out on the server side, directly within the request process. The backend tasks of data storage and management are taken care of by the system, while the user can concentrate on the research itself.

Copernicus Data Space Ecosytem supports several API families. OGC API-s directly enable the creation of Open Geospatial Consortium compatible map products such as WMS, WMTS, WFS or WCS services. These can be accessed with GIS software or displayed in web map tools. OData, STAC, and OpenSearch are Catalog API-s, supporting the querying and of datasets in preparation for analysis. Sentinel Hub is an API family that can handle queries, raster operations, and raster-vector integration for deriving statistics. The main advantages of Sentinel Hub API-s are their efficient use and integration with advanced visualization in the Copernicus Browser.

OpenEO is a fully open-source data analysis framework designed specifically to support FAIR principles. It is independent from data formats with its own data cube format, and can be edited using several coding languages. openEO connects to all STAC-compliant repositories, enabling integration between Sentinel data and other sources. Processing tools include many mathematical operations, but also standard machine learning processes. The system is designed with upscaling in mind: the command structure is the same for small and large areas, with storage and asynchronous processing managed by the backend.

Both API families come with a comprehensive scheme of tutorials and documentation to allow step-by-step learning, and an online Jupyter Lab virtual machine facility. Therefore, early-career scientists with a basic understanding of programming can quickly learn to apply their domain knowledge, while creating solutions that are easy to share and replicate.

All in all, Copernicus Data Space Ecosystem is a transformative tool for earth observation, significantly lowering the bar for applying earth observation at large scale in the geosciences.

How to cite: Zlinszky, A. and Milcinski, G.: Copernicus Data Space Ecosystem empowers early-career scientists to do global scale earth observation data analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15282, https://doi.org/10.5194/egusphere-egu25-15282, 2025.

EGU25-15672 | ECS | Posters on site | ESSI2.13

Scaling Down ESS Datasets: Lessons from the EERIE Project on Compression 

Oriol Tinto, Xavier Yepes, and Pierre Antoine Bretonniere

The rapid growth of Earth System Sciences (ESS) datasets, driven by high-resolution numerical modeling, has outpaced storage and data-sharing capabilities. To address these challenges, we investigated lossy compression techniques as part of the EERIE project, aiming to significantly reduce storage demands while maintaining the scientific validity of critical diagnostics.

Our study examined two key diagnostics: Sea Surface Height (SSH) variability and ocean density, essential for understanding climate dynamics. Leveraging tools such as SZ3 and enstools-compression, we achieved data volume reductions by orders of magnitude without compromising the diagnostics' accuracy. Compression-induced differences were found to be negligible compared to the inherent variability between model outputs and observational datasets, underscoring the robustness of these methods.

Additionally, our work highlighted inefficiencies in current workflows, including the prevalent use of double precision in post-processing. We proposed improvements to align data precision with the original model outputs, further optimizing storage and computation. Integrating lossy compression into existing workflows via widely used formats like NetCDF and HDF5 demonstrates a practical path forward for sustainable ESS data management.

This study showcases the transformative potential of lossy compression to make high-resolution datasets more manageable, ensuring they remain accessible and scientifically reliable for stakeholders while significantly reducing resource demands.

How to cite: Tinto, O., Yepes, X., and Bretonniere, P. A.: Scaling Down ESS Datasets: Lessons from the EERIE Project on Compression, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15672, https://doi.org/10.5194/egusphere-egu25-15672, 2025.

EGU25-15864 | Posters on site | ESSI2.13

The Sentinels EOPF Toolkit: Driving Community Adoption of the Zarr data format for Copernicus Sentinel Data 

Sabrina H. Szeto, Julia Wagemann, Emmanuel Mathot, and James Banting

The Standard Archive Format for Europe (SAFE) specification has been the established approach to publishing Copernicus Sentinel data products for over a decade. While SAFE has pushed the ecosystem forward through new ways to search and access the data, it is not ideal for processing large volumes of data using cloud computing. Over the last few years, data standards like STAC and cloud-native data formats like Zarr and COGs have revolutionised how scientific communities work with large-scale geospatial data and are becoming a key component of new data spaces, especially for cloud-based systems.

The ESA Copernicus Earth Observation Processor Framework (EOPF) will be providing access to “live” sample data from the Copernicus Sentinel missions -1, -2 and -3 in the new Zarr data format. This set of reprocessed data allows users to try out accessing and processing data in the new format and experiencing the benefits thereof with their own workflows.

This presentation introduces a community-driven toolkit that facilitates the adoption of the Zarr data format for Copernicus Sentinel data. The creation of this toolkit was driven by several motivating questions: 

  • What common challenges do users face and how can we help them overcome them? 
  • What resources would make it easier for Sentinel data users to use the new Zarr data format? 
  • How can we foster a community of users who will actively contribute to the creation of this toolkit and support each other?

The Sentinels EOPF Toolkit team, comprising Development Seed, SparkGeo and thriveGEO, together with a group of champion users (early-adopters), are creating a set of Jupyter Notebooks and plug-ins that showcase the use of Zarr format Sentinel data for applications across multiple domains. In addition, community engagement activities such as a notebook competition and social media outreach will bring Sentinel users together and spark interaction with the new data format in a creative yet supportive environment. Such community and user adoption efforts are necessary in order to overcome adoption and uptake barriers and to build up trust and excitement to try out new technologies and new developments around data spaces.

In addition to introducing the Sentinels EOPF Toolkit, this presentation will also highlight lessons learned from working closely with users on barriers they face in adopting the new Zarr format and how to address them. 

How to cite: Szeto, S. H., Wagemann, J., Mathot, E., and Banting, J.: The Sentinels EOPF Toolkit: Driving Community Adoption of the Zarr data format for Copernicus Sentinel Data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15864, https://doi.org/10.5194/egusphere-egu25-15864, 2025.

EGU25-16791 | ECS | Posters on site | ESSI2.13

Development and performance evaluation of dissolved oxygen climatology in the Northwestern Pacific 

Jae-Ho Lee, Yong Sun Kim, and Sung-Dae Kim

This study developed a monthly regional atlas for dissolved oxygen (DO) with a quarter-degree horizontal resolution and 73 vertical levels over the northwestern Pacific. We used observed profiles of 586,851 and gridded World Ocean Atlas 2023 (WOA23) with 1° resolution by adopting simple kriging horizontal interpolation and vertical stabilizing techniques to produce the new atlas. This approach efficiently mitigates artificial water masses and statistical noise. The new DO climatology provides detailed information along coasts and renders realistic oxygen distribution associated with the current system in the western North Pacific compared to WOA23. A meridional section demonstrates that the newly developed atlas does not yield artificial noise-like spikes frequently observed in WOA23 in the East Sea. This study expects that this new atlas can allow bio-geochemical numerical models to enhance diagnostic and forecasting performance.

How to cite: Lee, J.-H., Kim, Y. S., and Kim, S.-D.: Development and performance evaluation of dissolved oxygen climatology in the Northwestern Pacific, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16791, https://doi.org/10.5194/egusphere-egu25-16791, 2025.

EGU25-17102 | Posters on site | ESSI2.13

Calculation of Gridded Surface Current from Observed Lagrangian Trajectories in the East Sea 

Mi-Jin Jang, Jae-Ho Lee, and Yong Sun Kim

Surface ocean current is crucial for enhancing the safety and efficiency of maritime logistics and transportation, boosting fisheries production and management, and supporting military operations. This study analyzed 25,342 trajectories from NOAA’s Global Drifter Program (1991–2020), 12 from KIOST, and 63 from KHOA (2015–2024). The surface drifters entering the East Sea were extracted, and a five-step quality control process was implemented. Unobserved values were removed, quality control was applied based on drogue lost, abnormally speed or stuck, unrealistic acceleration. To estimated the gridded oceanic current with high-resolution, we removed the Ekman current and tides from the observed velocity and took advantage of a simple kriging approach. The validation against existing datasets confirmed that major ocean currents exhibited similar patterns compared to absolute geostrophic current from the satellite-based altimetry. The constructed dataset is expected to contribute to the accurate identification of surface current movements and the development of realistic models that incorporate regional characteristics based on data assimilation.

How to cite: Jang, M.-J., Lee, J.-H., and Kim, Y. S.: Calculation of Gridded Surface Current from Observed Lagrangian Trajectories in the East Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17102, https://doi.org/10.5194/egusphere-egu25-17102, 2025.

The Copernicus Program is the largest and most successful public space program globally. It provides continuous data across various spectral ranges, with an archive exceeding 84 petabytes and a daily growth of approximately 20 TB, both of which are expected to increase further. The openness of its data has contributed to the widespread use of Earth observation and the development of commercial products utilizing open data in Europe and worldwide. The entire archive, along with cloud-based data processing capabilities, is available free of charge through the Copernicus Data Space Ecosystem initiative and continues to evolve to meet global user standards. 

This paper presents the process of creating the STAC Copernicus Data Space Ecosystem catalog—the largest and most comprehensive STAC catalog in terms of metadata globally. It details the workflow, starting from the development of a metadata model for Sentinel data, through efficient indexing based on the original metadata files accompanying the products, to result validation and backend system ingestion (via database DSN). A particular highlight is that this entire process is executed using a single tool, eometadatatool, initially developed by DLR, further enhanced, and released as open-source software by the CloudFerro team. The eometadatatool facilitates metadata extraction from the original files accompanying Copernicus program products and others (e.g., Landsat, Copernicus Contributing Missions) using a CSV file containing the metadata name, the file in which it occurs, and the path to the key within the file. Since the CDSE repository operates as an S3 resource offering users free access, the tool supports product access via S3 resources by default, configurable through environment variables. All the above characterizes eometadatatool as the most powerful stactool (a high-level command-line tool and Python library for working with STAC) package available, providing both valid STAC items and a method for uploading them to the selected backend. 

The standard specification itself has been influenced by the CDSE catalog development process, which contributed to the evolution of the standard by introducing version 1.1 and updated extensions (storage, eo, proj) that better meet user needs. The paper discusses the most significant modifications, their impact on the catalog’s functionality, and outlines the main differences. 

Particular attention is given to performance optimization due to the substantial data volume and high update frequency. The study examines the configuration and performance testing (using Locust) of the frontend layer (stac-fastapi-pgstac) and backend (pgstac). The stac-fastapi-pgstac implementation was deployed on a scalable Kubernetes cluster and underwent a product hydration process (specific to managing JSON data in pgstac), leveraging Python's native capabilities for this task. The pgstac schema was deployed on a dedicated bare-metal server with a PostgreSQL database, utilizing master-worker replication enabled through appropriate pgstac configuration. Both software tools are open source, and the achieved optimal configurations are documented and will be presented in detail. 

The presented solution empowers the community to fully utilize the new catalog, leverage its functionalities, and access open tools that enable independent construction of STAC catalogs compliant with ESA and community recommendations. 

How to cite: Niemyjski, M. and Musiał, J.: Building the Copernicus Data Space Ecosystem STAC Catalog: Methodologies, Optimizations, and Community Impact, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17171, https://doi.org/10.5194/egusphere-egu25-17171, 2025.

EGU25-17172 | ECS | Orals | ESSI2.13

Neural Embedding Compression for Earth Observation Data – an Ablation Study 

Amelie Koch, Isabelle Wittmann, Carlos Gomez, Rikard Vinge, Michael Marszalek, Conrad Albrecht, and Thomas Brunschwiler

The exponential growth of Earth Observation data presents challenges in storage, transfer, and processing across fields such as climate modeling, disaster response, and agricultural monitoring. Efficient compression algorithms—either lossless or lossy—are critical to reducing storage demands while preserving data utility for specific applications. Conventional methods, such as JPEG and WebP, rely on hand-crafted base functions and are widely used. However, Neural Compression, a data-driven approach leveraging deep neural networks, has demonstrated superior performance by generating embeddings suitable for high levels of entropy encoding, enabling more accurate reconstructions at significantly lower bit rates.

In our prior work, we developed a Neural Compression pipeline utilizing a masked auto-encoder, embedding quantization, and an entropy encoder tailored for satellite imagery [1]. Instead of reconstructing original images, we evaluated the reconstructed embeddings for downstream tasks such as image classification and semantic segmentation. In this study, we conducted an ablation analysis to quantify the contributions of individual pipeline components—encoder, quantizer, and entropy encoder—toward the overall compression rate. Our findings reveal that satellite images achieve higher compression rates compared to ImageNet samples due to their lower entropy. Furthermore, we demonstrate the advantages of learned entropy models over hand-crafted alternatives, achieving better compression rates, particularly for datasets with seasonal or geospatial coherence. Based on these insights, we provide a list of recommendations for optimizing Neural Compression pipelines to enhance their performance and efficiency.

This work was conducted under the Embed2Scale project, supported by the Swiss State Secretariat for Education, Research and Innovation (SERI contract no. 24.00116) and the European Union (Horizon Europe contract no. 101131841).

[1] C. Gomes and T. Brunschwiler, “Neural Embedding Compression for Efficient Multi-Task Earth Observation Modelling,” IGARSS 2024, Athens, Greece, 2024, pp. 8268-8273, doi: 10.1109/IGARSS53475.2024.10642535.

How to cite: Koch, A., Wittmann, I., Gomez, C., Vinge, R., Marszalek, M., Albrecht, C., and Brunschwiler, T.: Neural Embedding Compression for Earth Observation Data – an Ablation Study, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17172, https://doi.org/10.5194/egusphere-egu25-17172, 2025.

EGU25-17326 | Orals | ESSI2.13

The UK EO DataHub - a pathfinder programme to develop a data space for UK industry, public and academic sectors 

Philip Kershaw, Rhys Evans, Fede Moscato, Dave Poulter, Alex Manning, Jen Bulpett, Ed Williamson, John Remedios, Alastair Graham, Daniel Tipping, and Piotr Zaborowski

The EO DataHub is a new national data space which has been under development as part of a two-year pathfinder programme to facilitate the greater exploitation of EO data for UK industry, public sector and academia. The project has been led by the UK National Centre for Earth Observation partnered with public sector bodies, the UK Space Agency, Met Office, Satellite Applications Catapult and National Physical Laboratory and enlisting commercial suppliers for the development and delivery of the software.

The Hub joins a crowded space in this sector as it joins a growing number of similar such platforms. However, as a national platform (with government as an anchor tenant) it is seeking to provide a unique offering as a trusted source of data, integrating curated data products from the science community building on UK strengths in climate research.

The architecture can be considered as a three layer model. At the base layer, different data sources are integrated - both commercial (Airbus and Planet Labs) and academic providers - from the CEDA data archive (https://archive.ceda.ac.uk) hosted on the JASMIN supercomputer (https://jasmin.ac.uk). The data catalogue now includes high and very high resolution SAR and optical products, Sentinel, UK Climate Projections, CMIP (https://wcrp-cmip.org), CORDEX (https://cordex.org) and outputs from EOCIS (https://eocis.org) consisting of a range of satellite-derived climate data products.

The middle layer, the Hub Platform provides services and APIs including federated search which integrates the data from the various providers, image visualisation, a workflow engine, user workspaces and interactive analysis environments. These build on the work of ESA's EOEPCA (https://eoepca.org) and apply open standards from the Open Geospatial Consortium and STAC (https://stacspec.org/) for cataloguing. In providing this suite of services, the goal is to provide a toolkit to facilitate application developers and EO specialists in building new applications and tools to exploit the data. This forms the final layer in the architecture: as part of the programme, three example application scenarios have been funded, each partnered with a target set of users. These include 1) an application taking climate projections and land surface temperature datasets to provide risk assessments for land assets (led by SparkGeo); 2) a land cover application (Spyrosoft) and finally 3), rather than an application in its own right, a project to develop a client toolkit for use with Jupyter Notebooks and a plugin integrating the Hub’s functionality into the open source GIS desktop application QGIS (work led by Oxidian).

Over the course of the programme, running in parallel to the system development, a dedicated study has been undertaken to develop a model for future sustainability of the platform tackling engagement with potential users and cost models. At the beginning, a funding call seeded early pilots to investigate application scenarios that the platform could support. As this initial phase of the Hub completes, work is underway to engage with early adopters and provide training resources for new users.

How to cite: Kershaw, P., Evans, R., Moscato, F., Poulter, D., Manning, A., Bulpett, J., Williamson, E., Remedios, J., Graham, A., Tipping, D., and Zaborowski, P.: The UK EO DataHub - a pathfinder programme to develop a data space for UK industry, public and academic sectors, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17326, https://doi.org/10.5194/egusphere-egu25-17326, 2025.

EGU25-17799 | Posters on site | ESSI2.13

Data Spaces and geodata workflows for environmental protection 

Matthes Rieke, Benjamin Proß, Simon Jikra, Sotiris Aspragkathos, Iasonas Sotiropoulos, Stamatia Rizou, and Lisa Pourcher

The concept of Data Spaces has gained traction in recent years. Major representatives emerged which have the technological maturity as well as support by relevant decision and policy makers (e.g.  the International Data Spaces Association (IDSA) or Gaia-X). These follow different architectural approaches. In this session we want to illustrate the challenges of integrating the Data Space architectures with established concepts of Spatial Data Infrastructure.

During the next 4 years, the ENFORCE project (Empower citizeNs to join Forces with public authORities in proteCting the Environment) is dedicated to fostering sustainable practices and ensuring environmental regulatory compliance by integrating citizen science with innovative technologies. By employing Living Labs and citizen science methodologies, ENFORCE will create innovative tools that bridge the gap between data reporting, monitoring, and policy enforcement. The project integrates data collection (e.g. Copernicus satellite data), analysis, and stakeholder participation to meet these goals. ENFORCE will leverage geospatial intelligence and explainable AI to enhance environmental governance. These tools and strategies will be tested and refined at eight pilot sites in seven countries, supplemented by capacity-building and policy recommendation efforts.

The design and development of a geospatial information infrastructure that supports the envisioned data workflows is a key challenge addressed by ENFORCE. This infrastructure will prioritize the integration of OGC API-driven systems into the Data Space ecosystem, forming a central component of the project’s agenda. Through development of a blueprint architecture for integration, the project will identify gaps and missing components in current systems, aligning with standards such as the FAIR principles and open data. The concepts will be facilitated in an ENFORCE “Tools Plaza”, an innovative platform providing data science and analytical capabilities for environmental compliance workflows.

How to cite: Rieke, M., Proß, B., Jikra, S., Aspragkathos, S., Sotiropoulos, I., Rizou, S., and Pourcher, L.: Data Spaces and geodata workflows for environmental protection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17799, https://doi.org/10.5194/egusphere-egu25-17799, 2025.

EGU25-19418 | Posters on site | ESSI2.13

Lossy Data Compression Exploration in an Online Laboratory and the Link to HPC Design Decisions 

Karsten Peters-von Gehlen, Juniper Tyree, Sara Faghih-Naini, Peter Dueben, Jannek Squar, and Anna Fuchs

It is apparent that the data amounts expected to be generated by current and upcoming Earth System Science research and operational activities stress the capabilities of HPC and associated data infrastructures. Individual research projects focusing on running global Earth System Models (ESMs) at spatial resolution of 5km or less can easily occupy several petabytes on disk. With multiple of such projects running on a single HPC infrastructure, the challenge of storing the data alone becomes apparent. Further, community-driven activities like model intercomparison projects – which are conducted for both conventional and high-resolution model setups – add to the aforementioned strain on storage systems. Hence, when planning for next-generation HPC systems, the storage requirements of state-of-the-art ESM-centered projects have to be clear so that systems are still fit-for-use 5 years down the road from the initial planning stage.

As computational hardware costs per performance unit (FLOP or Byte) are not decreasing anymore like they have in the past decades, HPC system key figures do not increase substantially anymore from one generation to the next. The mismatch between demands of research and what future systems can offer is therefore clear.

One apparent solution to this problem is to simply reduce the amount of data from ESM simulations stored on a system. Data compression is one candidate to achieve this. Current ESM projects already utilize application-side lossless compression techniques, which help reduce storage space. However, decompression may incur performance penalties, especially when read patterns misalign with the compression block sizes. Lossy compression offers the potential for higher compression rates, without access penalties for data retrieval. However, its suitability is highly content-dependent, raising questions about which lossy compression methods are best suited for specific datasets. On a large scale, applying lossy compression also prompts the consideration of how such data reduction could shape the design of next-generation HPC architectures.

With lossy compression not being very popular in the ESM-community so far, we present a key development of the ongoing ESiWACE3 project: an openly accessible Jupyter-based online laboratory for testing lossy compression techniques on ESM output datasets. This online tool currently comes with a set of notebooks allowing users to objectively evaluate the impact lossy compression has on analyses performed on the compressed compared to the input data. With some compressors promising compression ratios of 10x-1000x, providing such tools to ensure compression quality is essential. The motivation behind the online compression laboratory is to foster the acceptance of lossy compression techniques by conveying first-hand experience and immediate feedback of benefits or drawbacks of applying lossy compression algorithms. 

Going one step further, we illustrate the impacts that applying lossy-compression techniques on ESM data on large-scales can have on the design decisions made for upcoming HPC infrastructures. We illustrate, among others, that increased acceptance and application of lossy compression techniques enables more efficient resource utilization and allows for smarter reinvestment of funds saved from reduced storage demands, potentially leading to the acquisition of smaller systems and thus enabling increased research output per resource used.

How to cite: Peters-von Gehlen, K., Tyree, J., Faghih-Naini, S., Dueben, P., Squar, J., and Fuchs, A.: Lossy Data Compression Exploration in an Online Laboratory and the Link to HPC Design Decisions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19418, https://doi.org/10.5194/egusphere-egu25-19418, 2025.

EGU25-20188 | ECS | Posters on site | ESSI2.13

Creating TROPOMI superobservations for data assimilation and model evaluation 

Pieter Rijsdijk, Henk Eskes, Kazuyuki Miyazaki, Takashi Sekiya, and Sander Houweling

Satellite observations of tropospheric trace gases and aerosols are evolving rapidly. Recently launched instruments provide increasingly higher spatial resolutions with footprint diameters in the range of 2–8 km, with daily global coverage for polar orbiting satellites or hourly observations from geostationary orbit. Often the modelling system has a lower spatial resolution than the satellites used, with a model grid size in the range of 10–100 km. When the resolution mismatch is not properly bridged, the final analysis based on the satellite data may be degraded. Superobservations are averages of individual observations matching the resolution of the model and are functional to reduce the data load on the assimilation system. In this paper, we discuss the construction of superobservations, their kernels and uncertainty estimates. The methodology is applied to nitrogen dioxide tropospheric column measurements of the TROPOMI instrument on the Sentinel-5P satellite. In particular, the construction of realistic uncertainties for the superobservations is non-trivial and crucial to obtaining close to optimal data assimilation results. We present a detailed methodology to account for the representativity error when satellite observations are missing due to e.g. cloudiness. Furthermore, we account for systematic errors in the retrievals leading to error correlations between nearby individual observations contributing to one superobservation. Correlation information is typically missing in the retrieval products where an error estimate is provided for individual observations. The various contributions to the uncertainty are analysed: from the spectral fitting, the estimate of the stratospheric contribution to the column and the air-mass factor. The method is applied to TROPOMI data but can be generalised to other trace gases such as HCHO, CO, SO2 and other instruments such as OMI, GEMS and TEMPO. The superobservations and uncertainties are tested in the ensemble Kalman filter chemical data assimilation system developed by JAMSTEC. These are shown to improve forecasts compared to thinning or compared to assuming fully correlated or uncorrelated uncertainties within the superobservation. The use of realistic superobservations within model comparisons and data assimilation in this way aids the quantification of air pollution distributions, emissions and their impact on climate.

How to cite: Rijsdijk, P., Eskes, H., Miyazaki, K., Sekiya, T., and Houweling, S.: Creating TROPOMI superobservations for data assimilation and model evaluation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20188, https://doi.org/10.5194/egusphere-egu25-20188, 2025.

EGU25-20430 | Orals | ESSI2.13

Compression and Aggregation: a CF data model approach 

David Hassell, Sadie Bartholomew, Bryan Lawrence, and Daniel Westwood

The CF (Climate and Forecast) metadata conventions for netCDF datasets describe means of "compression-by-convention", i.e. methods for compressing and decompressing data according to algorithms that are fully described within the conventions themselves. These algorithms, which can be lossless or lossy, are not applicable to arbitrary data, rather the data have to exhibit certain characteristics to make the compression worthwhile, or even possible.

Aggregation, available in CF-1.13, provides the utility of being able to view, as a single entity, a dataset that has been partitioned across multiple other independent datasets on disk, whilst taking up very little extra space on disk since the aggregation dataset contains no copies of the data in each component dataset. Aggregation can facilitate a range of activities such as data analysis, by avoiding the computational expense of deriving the aggregation at the time of analysis; archive curation, by acting as a metadata-rich archive index; and the post-processing of model simulation outputs, by spanning multiple datasets written at run time that together constitute a more cohesive and useful product. CF aggregation currently has cf-python and xarray implementations.

The conceptual CF data model does not recognise compression nor aggregation, choosing to view all CF datasets as if they were uncompressed and containing all of their own data. As a result, the cf-python data analysis library, that is built exactly on the CF data model, also presents datasets lazily to the user in this manner, without decompressing or re-combining the data in memory until the user actually accesses the data, at which time it occurs automatically. This approach allows the user to interact with their data in an intuitive and efficient manner; and also removes the need for the user to have to assimilate large parts of the CF conventions and having to create their own code for dealing with the compression and aggregation algorithms.

We will introduce compression by ragged arrays (as used by Discrete Sampling Geometry features, such as timeseries and trajectories) and dataset aggregation, with cf-python examples to demonstrate the ease of use that arises from using the CF data model interpretation of the data.

How to cite: Hassell, D., Bartholomew, S., Lawrence, B., and Westwood, D.: Compression and Aggregation: a CF data model approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20430, https://doi.org/10.5194/egusphere-egu25-20430, 2025.

EGU25-1511 | ECS | Orals | ESSI3.3

A workflow for cloud-based and HPC simulations with the NEMO ocean model using containers 

Aina Gaya-Àvila, Bruno de Paula Kinoshita, Stella V. Paronuzzi Ticco, Oriol Tintó Prims, and Miguel Castrillo

In this work, we explored the deployment and execution of the NEMO ocean model using Singularity containers within the EDITO Model Lab, implementing the European Digital Twin of the Ocean. The Auto-NEMO workflow, a fork of Auto-EC-Earth used to run NEMO workflows using the NEMO Community reference code, was adapted to run simulations using containers. The use of a Singularity container ensures consistent execution by packaging all dependencies, making it easier to deploy the model across various HPC systems.

The containerized approach was tested on multiple HPC platforms, including MareNostrum5 and LUMI, to evaluate scaling performance. Our tests compared the use of mpich and openmp libraries, providing insights into how communication strategies impact the computational performance of the model in containerized setups. In addition, the runs are orchestrated by a content workflow manager, in this case Autosubmit, deployed in a cloud infrastructure in EDITO-Infra, making the entire solution (workflow manager and workflow itself) portable end-to-end. The benefits of portability and reproducibility make containers an attractive solution for streamlining workflows in diverse computational environments.

A comparison between containerized and non-containerized runs highlights the trade-offs involved. Direct execution may provide slightly better performance in some cases, but the containerized approach greatly reduces setup complexity. These findings demonstrate the potential of containerization to enhance efficiency and accessibility in large-scale ocean modeling efforts.

How to cite: Gaya-Àvila, A., de Paula Kinoshita, B., Paronuzzi Ticco, S. V., Tintó Prims, O., and Castrillo, M.: A workflow for cloud-based and HPC simulations with the NEMO ocean model using containers, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1511, https://doi.org/10.5194/egusphere-egu25-1511, 2025.

EGU25-2142 | ECS | Posters on site | ESSI3.3

Enhancing Data Provenance in Workflow Management: Integrating FAIR Principles into Autosubmit and SUNSET 

Albert Puiggros, Miguel Castrillo, Bruno de Paula Kinoshita, Pierre-Antoine Bretonniere, and Victòria Agudetse

Ensuring robust data provenance is paramount for advancing transparency, traceability, and reproducibility in climate research. This work presents the integration of FAIR (Findable, Accessible, Interoperable, and Reusable) principles into the workflow management ecosystem through provenance integration in Autosubmit, a workflow manager developed at the Barcelona Supercomputing Center (BSC), and SUNSET (SUbseasoNal to decadal climate forecast post-processing and asSEmenT suite), an R-based verification workflow also developed at the BSC.

Autosubmit supports the generation of data provenance information based on RO-Crate, facilitating the creation of machine-actionable digital objects that encapsulate detailed metadata about its executions. Autosubmit integrates persistent identifiers (PIDs) and schema.org annotations, making provenance records more accessible and actionable for both humans and machines.  However, the provenance metadata provided by Autosubmit through RO-Crate focuses on the workflow process and does not encapsulate the details of the data transformation processes. This is where SUNSET plays a complementary role. SUNSET’s approach for provenance information is based on the METACLIP (METAdata for CLImate Products) ontologies. METACLIP offers a semantic approach for describing climate products and their provenance. This framework enables SUNSET to provide specific, high-resolution  provenance metadata for its operations, improving transparency and compliance with FAIR principles. The generated files provide detailed information about each transformation the data has undergone, as well as additional details about the data's state, location, structure, and associated source code, all represented in a tree-like structure.

The main contribution of this work is the generation of a comprehensive provenance object by integrating these tools. SUNSET uses Autosubmit to parallelize its data processing tasks, with Autosubmit managing SUNSET jobs. As part of this process, an RO-Crate is automatically generated describing the overall execution. This object encapsulates detailed provenance metadata for each individual job within the workflow, using METACLIP's semantic framework to represent each SUNSET execution process. Certain schema.org entities are introduced to have the RO-Crate created by Autosubmit link with the provenance details generated by SUNSET. This integrated approach provides a unified hierarchical provenance record that spans to both the workflow management system and the individual job executions, ensuring that provenance objects are automatically generated for each experiment conducted.

This work demonstrates the practical application of FAIR principles in climate research by advancing provenance tracking within complex workflows. It represents an initial step to obtain and share metadata about the provenance of the data products that a workflow provides. The integration of RO-Crate and METACLIP not only enhances the reproducibility of climate data products but also fosters greater confidence in their reliability. To our knowledge, this is the first effort in the climate domain to combine different provenance formats into a single object, aiming to obtain a complete provenance graph with all the metadata. 

How to cite: Puiggros, A., Castrillo, M., de Paula Kinoshita, B., Bretonniere, P.-A., and Agudetse, V.: Enhancing Data Provenance in Workflow Management: Integrating FAIR Principles into Autosubmit and SUNSET, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2142, https://doi.org/10.5194/egusphere-egu25-2142, 2025.

EGU25-4355 | ECS | Posters on site | ESSI3.3

Generic State Vector: streaming and accessing high resolution climate data from models to end users 

Iker Gonzalez-Yeregi, Pierre-Antoine Bretonnière, Aina Gaya-Avila, and Francesc Roura-Adserias

The Climate Adaptation Digital Twin (ClimateDT) is a contract under the Destination Earth initiative (DestinE) that aims to develop a digital twin to account for climate change adaptation. This is achieved by running high-resolution simulations with different climate models by making use of the different EuroHPC platforms. In addition to the climate models, applications that consume data from models are also developed under the contract. A common workflow is used to execute the whole pipeline from the model launching to the data consumption by the applications in a user-friendly and automated way.

One of the challenges of this complex workflow is to handle the different outputs that each of the climate models initially offered. Each model works with its own grid, vertical levels, and variable set. These differences in format make it very complicated for applications to consume and compare data coming from different models in an automated and timely manner. This issue is resolved by introducing the concept of Generic State Vector (GSV), which defines a common output portfolio for all models to ensure a homogeneous output between models. The conversion from the model's native output to the GSV happens before the data is written in the HPC and it is automated in the workflow allowing transparent access to the data changing only the name of the model in the call.

Data in the GSV format can be read using a newly designed dedicated Python tool: the GSV Interface. This tool links the model part of the workflow with the applications part of the workflow, enabling running everything in a single complex workflow (end-to-end workflow). The GSV Interface allows to read data that has been previously converted to GSV, adding proper metadata. It also offers some extra features like interpolation to regular grids and area selection. All the workflow components that read data from the models rely on the GSV Interface. In addition to that, the GSV Interface can also be used to transparently retrieve and process data from the public Destination Earth Service Platform.

How to cite: Gonzalez-Yeregi, I., Bretonnière, P.-A., Gaya-Avila, A., and Roura-Adserias, F.: Generic State Vector: streaming and accessing high resolution climate data from models to end users, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4355, https://doi.org/10.5194/egusphere-egu25-4355, 2025.

EGU25-4466 | ECS | Posters on site | ESSI3.3

ClimateDT Workflow: A containerized climate workflow 

Francesc Roura-Adserias, Aina Gaya-Avila, Leo Arriola i Meikle, Iker Gonzalez-Yeregi, Bruno De Paula Kinoshita, Jaan Tollander de Balsch, and Miguel Castrillo

The Climate Adaptation Digital Twin (ClimateDT), a contract (DE_340) inside the Destination Earth (DestinE) flagship initiative from the European Commission, is a highly collaborative project where climate models are executed in an operational manner on different EuroHPC platforms. The workflow software supporting such executions, called ClimateDT Workflow, contains a model component and an applications component. The applications can be seen as elements that consume the data that is provided by the climate models. They aim to provide climate information to sectors that are critically dependent on climate change, such as renewable energy or wildfires, among others. This workflow relies on the Autosubmit workflow manager and is executed over different EuroHPC platforms that are part of the contract.

There are six lightweight applications that are run in this workflow, in parallel to the model and in a streaming fashion. Setting up and maintaining an environment for these applications for each EuroHPC platform (plus the development environments) is a time-consuming and cumbersome task. These machines are shared by multiple users, have different operating systems and libraries, some do not have internet access for all users on their login nodes, and there are different rules to install and maintain software on each machine.

In order to overcome these difficulties all the application-required dependencies of the workflow are encapsulated beforehand in a Singularity container and therefore the portability to the different platforms becomes merely an issue with path-binding inside the platform. Through the use of Singularity containers, their execution does not require administrator permissions, which allows anyone with access to the project to execute the desired application either on the EuroHPC machines, or on their local development environment.

This work shows the structure of the ClimateDT workflow and how it uses Singularity containers, how they contribute not only to portability but also to traceability and provenance, and finally the benefits and issues found during its implementation. We believe that the successful use of containers in this climate workflow, where applications run in parallel to the climate models in a streaming fashion and where the complete workflow runs on different HPC platforms, presents a good reference for other projects and workflows that must be platform-agnostic and that require agile portability of their components.

How to cite: Roura-Adserias, F., Gaya-Avila, A., Arriola i Meikle, L., Gonzalez-Yeregi, I., De Paula Kinoshita, B., Tollander de Balsch, J., and Castrillo, M.: ClimateDT Workflow: A containerized climate workflow, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4466, https://doi.org/10.5194/egusphere-egu25-4466, 2025.

In an era of unprecedented availability of Earth Observation (EO) data, the Copernicus Data Space Ecosystem (CDSE) emerges as a vital platform to bridge the gap between data accessibility and actionable insights. With petabytes of freely accessible satellite data at our fingertips and multiple operational data processing platforms in place, many of the foundational challenges of accessing and processing sensor data have been addressed. Yet, the widespread adoption of EO-based applications remains below expectations. The challenge lies in the effective extraction of relevant information from the data. While numerous R&D projects demonstrate the possibilities of EO, their results are often neither repeatable nor reusable, primarily due to prototype-level implementations and overly tailored, non-standardized workflows.  

CDSE tackles these barriers by adopting common standards and patterns, most notably through openEO, an interface designed to standardize EO workflow execution across platforms. openEO enables the development of reusable workflows that are scalable and transferable, paving the way for systematic and objective monitoring of the planet. CDSE has already integrated openEO as a core processing interface, and further advancements are underway, including the integration of Sentinel Hub to support openEO. This integration will enhance instantaneous visualization, synchronous API requests, and batch processing, as well as support openEO process graphs within the Copernicus Browser, bringing the simplicity and speed of Sentinel Hub’s synchronous engine to the openEO ecosystem.  

CDSE’s openEO capabilities are already validated through large-scale operational projects such as ESA WorldCereal and Copernicus Global Land Cover and Tropical Forestry Mapping and Monitoring Service (LCFM), which leverage its robust, scalable, and reliable infrastructure. Additionally, the openEO Algorithm Plaza fosters collaboration by enabling the easy sharing and reuse of processing workflows, while the Bring Your Own Data feature allows users to integrate their datasets into the ecosystem, promoting data interoperability and collaborative advancements.  

CDSE is embracing a federated approach, allowing additional data or service providers to become part of the ecosystem. This inclusivity ensures a growing network of interoperable services while maintaining technical and operational stability—a cornerstone for broad adoption and long-term sustainability.  

By addressing the need for operational and reusable workflows with openEO and related initiatives, CDSE is not only advancing the technical landscape of EO but also fostering a culture of repeatable, scalable, and impactful science. Through this session, we aim to spark a discussion on how to make EO applications more accessible, reusable, and impactful for the global community.

How to cite: Sharma, P.: How openEO standardizes workflows for scalable and reusable EO data analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5593, https://doi.org/10.5194/egusphere-egu25-5593, 2025.

EGU25-6201 | Orals | ESSI3.3

Advancing Computational Workflow Sharing in Earth Science: Insights from DT-GEO and Geo-INQUIRE 

Marco Salvi, Rossana Paciello, Valerio Vinciarelli, Kety Giuliacci, Daniele Bailo, Pablo Orviz, Keith Jeffery, Manuela Volpe, Roberto Tonini, and Alejandra Guerrero

The increasing complexity and volume of data in Solid Earth Science necessitate robust solutions for workflow representation, sharing, and reproducibility. Within the DT-GEO (https://dtgeo.eu/) project, we addressed the challenge of creating interoperable and discoverable representations of computational workflows to facilitate data reuse and collaboration. Leveraging the EPOS Platform (https://www.epos-eu.org/), a multidisciplinary research infrastructure focused on Solid Earth Science, we aimed to expose workflows, datasets, and software to the community while adhering to the FAIR (Findable, Accessible, Interoperable, and Reusable) principles. While the EPOS-DCAT-AP (https://github.com/epos-eu/EPOS-DCAT-AP) model, already used in EPOS, can effectively represent datasets and software, it lacks direct support for computational workflows, necessitating the adoption of alternative standards.

To overcome this limitation, we employed the Common Workflow Language (CWL, https://www.commonwl.org/) to describe workflows, capturing their structure, software, datasets, and dependencies. The developed CWL representations are "abstract" focusing on general workflow structures while omitting execution-specific details to prioritize interoperability. To package these workflows along with metadata, we utilized Workflow Run Crate, an extension of the RO-Crate (https://www.researchobject.org/ro-crate/) standard. Together, these technologies enable workflows to become self-contained entities, simplifying sharing and reuse. 

This approach not only aligns with community standards but also benefits from a mature ecosystem of tools and libraries, ensuring seamless integration and widespread applicability. Initial implementations within the DT-GEO project serve as a model for adoption in related initiatives such as Geo-INQUIRE (https://www.geo-inquire.eu/), where similar methodologies are being used to share workflows derived from the Simulation Data Lake (SDL) infrastructure. These implementations pave the way for broader integration within the EPOS Platform, enhancing access to advanced workflows across disciplines.

Our contribution highlights the value of adopting standardized tools and methodologies for workflow management in Solid Earth Science, showcasing how CWL and RO-Crate streamline interoperability and foster collaboration. These advances address challenges in data and computational management, contributing to the scalable FAIR workflows essential for tackling the complexities of Solid Earth Science. Moving forward, the integration of these standards across projects like DT-GEO and Geo-INQUIRE will further enhance the EPOS Platform's capabilities, offering a unified gateway to reproducible, secure, and trustworthy workflows that meet the evolving needs of the scientific community.

How to cite: Salvi, M., Paciello, R., Vinciarelli, V., Giuliacci, K., Bailo, D., Orviz, P., Jeffery, K., Volpe, M., Tonini, R., and Guerrero, A.: Advancing Computational Workflow Sharing in Earth Science: Insights from DT-GEO and Geo-INQUIRE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6201, https://doi.org/10.5194/egusphere-egu25-6201, 2025.

EGU25-6216 | Posters on site | ESSI3.3

CAMELS-PLUS: Enhancing Hydrological Data Through FAIR Innovations. 

Carlos Zuleta Salmon, Mirko Mälicke, and Alexander Dölich

The CAMELS-PLUS initiative is revolutionizing the way hydrological, and Earth System Science (ESS) data are processed, shared, and utilized by enhancing the widely-used CAMELS-DE dataset. While Germany boasts one of the richest hydrological datasets globally, CAMELS-DE has faced challenges due to its reliance on fragmented, manual workflows, which are error-prone and hinder collaboration. CAMELS-PLUS introduces a groundbreaking solution: a standardized framework for containerized scientific tools that embed rich metadata, ensuring provenance, reusability, and seamless integration across diverse scientific domains.

A key innovation of CAMELS-PLUS lies in its ability to bridge the gap between disciplines by implementing a fully containerized pipeline for dataset pre-processing. This approach allows researchers in meteorology, forestry, and other ESS subdomains to easily contribute and extend CAMELS-DE without the complexity of navigating storage systems or inconsistent workflows. The initiative’s metadata schema, implemented as YAML files with JSON-based tool parameterization, enables tools to "speak the same language," ensuring they are interoperable and aligned with FAIR principles.

Key Deliverables:

  • Updated CAMELS-DE Dataset: Incorporates new precipitation sources and enhanced metadata for seamless integration with the NFDI4Earth Knowledge Hub.
  • Standardized Scientific Containers: A community-adopted specification for containerized tools, promoting accessibility and reusability across disciplines.
  • Interactive Community Engagement: Extensions to camels-de.org, transforming it into a hub for exploring workflows and fostering interdisciplinary collaboration.

What makes CAMELS-PLUS particularly compelling is its potential to democratize access to cutting-edge hydrological datasets. By enabling non-specialists to contribute and utilize CAMELS-DE through intuitive, containerized workflows, the initiative reduces barriers to entry and accelerates innovation in data-driven hydrology and beyond. This project not only sets a new standard for dataset management in ESS but also creates a replicable model for tackling similar challenges across other scientific domains. CAMELS-PLUS is poised to inspire transformative changes in how large-sample datasets are curated, shared, and advanced for global scientific impact.

How to cite: Zuleta Salmon, C., Mälicke, M., and Dölich, A.: CAMELS-PLUS: Enhancing Hydrological Data Through FAIR Innovations., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6216, https://doi.org/10.5194/egusphere-egu25-6216, 2025.

EGU25-6544 | Posters on site | ESSI3.3

PyActiveStorage:  Efficient distributed data analysis using Active Storage for HDF5/NetCDF4 

Bryan N. Lawrence, David Hassell, Grenville Lister, Predoi Valeriu, Scott Davidson, Mark Goddard, Matt Pryor, Stig Telfer, Konstantinos Chasapis, and Jean-Thomas Acquaviva

Active storage (also known as computational storage) has been a concept often proposed but not often delivered. The idea is that there is a lot of under-utilised compute power in modern storage systems, and this could be utilised to carry out some parts of data analysis workflows. Such a facillity would reduce the cost of moving data, and make distributed data analysis much more efficient.

For storage to be able to handle compute, either an entire compute stack has to be migrated to the storage (with all the problems around security and dependencies) or the storage has to offer suitable compute interfaces. Here we take the second approach, borrowing the concept of providing system reduction operations in the MPI interface of HPC systems, to define and implement a reduction interface for the complex layout of HDF5 (and NetCDF4) data.

We demonstrate a near-production quality deployment of the technology (PyActiveStorage) fronting JASMIN object storage, and describe how we have built a POSIX prototype. The first provides compute “near” the storage, the second is truly “in” the storage. The performance with the object store is such that for some tasks distributed workflows based on reduction operations on HDF5 data can be competitive with local workflow speeds, a result which has significant implications for avoiding expensive copies of data and unnecessary data movement. As a byproduct of this work, we have also upgraded a pre-existing pure python HDF5 reader to support lazy access, which opens up threadsafe read operations on suitable HDF5 and NetCDF4 data.

To our knowledge, there has previously been no previous practical demonstration of active storage for scientific data held in HDF5 files. While we have developed this technology with application in distributed weather and climate workflows, we believe it will find utility in a wide range of scientific workflows.

How to cite: Lawrence, B. N., Hassell, D., Lister, G., Valeriu, P., Davidson, S., Goddard, M., Pryor, M., Telfer, S., Chasapis, K., and Acquaviva, J.-T.: PyActiveStorage:  Efficient distributed data analysis using Active Storage for HDF5/NetCDF4, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6544, https://doi.org/10.5194/egusphere-egu25-6544, 2025.

EGU25-7056 | Orals | ESSI3.3

Reliable and reproducible Earth System Model data analysis with ESMValTool 

Valeriu Predoi and Bouwe Andela

ESMValTool is a software tool for analyzing data produced by Earth System Models (ESMs) in a reliable and reproducible way. It provides a large and diverse collection of “recipes” that reproduce standard, as well as state-of-the-art analyses. ESMValTool can be used for tasks ranging from monitoring continuously running ESM simulations to analysis for scientific publications such as the IPCC reports, including reproducing results from previously published scientific articles as well as allowing scientists to produce new analysis results. To make ESMValTool a user-friendly community tool suitable for doing open science, it adheres to the FAIR principles for research software. It is: - Findable - it is published in community registries, such as https://research-software-directory.org/software/esmvaltool; - Accessible - it can be installed from Python package community distribution channels such as conda-forge, and the open-source code is available on Zenodo with a DOI, and on GitHub; - Interoperable - it is based on standards: it works with data that follows CF Conventions and the Coupled Model Intercomparison Project (CMIP) Data Request, its reusable recipes are written in YAML, and provenance is recorded in the W3C PROV format. It supports diagnostics written in a number of programming language, with Python and R being best supported. Its source code follows the standards and best practices for the respective programming languages; - Reusable - it provides a well documented recipe format and Python API that allow reusing previous analyses and building new analysis with previously developed components. Also, the software can be installed from conda-forge and DockerHub and can be tailored by installing from source from GitHub. In terms of input data, ESMValTool integrates well with the Earth System Grid Federation (ESGF) infrastructure. It can find, download and access data from across the federation, and has access to large pools of observational datasets. ESMValTool is built around two key scientific software metrics: scalability and user friendliness. An important aspect of user friendliness is reliability. ESMValTool is built on top of the Dask library to allow scalable and distributed computing, ESMValTool also uses parallelism at a higher level in the stack, so that jobs can be distributed on any standard High Performance Computing (HPC) facility; and software reliability and reproducibility - our main strategy to ensure reliability is modular, integrated, and tested design. This comes back at various levels of the tool. We try to separate commonly used functionality from “one off” code, and make sure that commonly used functionality is covered by unit and integration tests, while we rely on regression testing for everything else. We also use comprehensive end-to-end testing for all our “recipes” before we release new versions. Our testing infrastructure ranges from basic unit tests to tools that smartly handle various file formats, and use image comparison algorithms to compare figures. This greatly reduces the need for ‘human testing’, allowing for built-in robustness through modularity, and a testing strategy that has been tailored to match the technical skills of its contributors.

How to cite: Predoi, V. and Andela, B.: Reliable and reproducible Earth System Model data analysis with ESMValTool, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7056, https://doi.org/10.5194/egusphere-egu25-7056, 2025.

EGU25-7070 | Posters on site | ESSI3.3

EarthCODE - a FAIR and Open Environment for collaborative research in Earth System Science  

Chandra Taposeea-Fisher, Garin Smith, Ewelina Dobrowolska, Daniele Giomo, Francesco Barchetta, Stephan Meißl, and Dean Summers

The Open Science and Innovation Vision included in ESA’s EO Science Strategy (2024) addresses 8 key elements: 1) openness of research data, 2) open-source scientific code, 3) open access papers with data and code; 4) standards-based publication and discovery of scientific experiments, 5) scientific workflows reproducible on various infrastructures, 6) access to education on open science, 7) community practice of open science; and 8) EO business models built on open-source. EarthCODE (https://earthcode.esa.int) is a strategic ESA EO initiative to support the implementation of this vision. 

EarthCODE (Earth Science Collaborative Open Development Environment) will form part of the next generation of cloud-based geospatial services, aiming towards an integrated, cloud-based, user-centric development environment for European Space Agency’s (ESA) Earth science activities. EarthCODE looks to maximise long-term visibility, reuse and reproducibility of the research outputs of such projects, by leveraging FAIR and open science principles and enabling, thus fostering a sustainable scientific process. EarthCODE proposes a flexible and scalable architecture developed with interoperable open-source blocks, with a long-term vision evolving by incrementally integrating industrially provided services from a portfolio of the Network of Resources.  Additionally, EarthCODE is a utilisation domain of EOEPCA+, contributing to the development and evolution of Open Standards and protocols, enabling internationally interoperable solutions.  

EarthCODE will provide an Integrated Development Platform, giving developers tools needed to develop high quality workflows, allowing experiments to be executed in the cloud and be end-to-end reproduced by other scientists. EarthCODE is built around existing open-source solutions, building blocks and platforms, such as the Open Science Catalogue, EOxHub and EOEPCA. It has additionally begun to integrate platform services from DeepESDL, Euro Data Cube, Polar TEP and the openEO federation on CDSE platforms, with more being added annually through ESA best practices. With it’s adopted federated approach, EarthCODE will facilitate processing on other platforms, i.e. DeepESDL, ESA EURO Data Cube, Open EO Cloud/Open EO Platform and AIOPEN/AI4DTE.   

The roadmap for the portal includes the initial portal release by end of 2024, followed by the capability to publish experiments in Q1 2025 (including development, publishing, finding and related community engagement), and by mid-2025 to have a further release with reproducibility capabilities around accessibility and execute functionalities.  

Collaboration and Federation are at the heart of EarthCODE. As EarthCODE evolves we expect providing solutions allowing federation of data and processing. EarthCODE has ambition to deliver a model for a Collaborative Open Development Environment for Earth system science, where researchers can leverage the power of the wide range of EO platform services available to conduct their science, while also making use of FAIR Open Science tools to manage data, code and documentation, create end-to-end reproducible workflows on platforms, and have the opportunity to discover, use, reuse, modify and build upon the research of others in a fair and safe way. Overall, EarthCODE aims to enable elements for EO Open Science and Innovation vision, including open data, open-source code, linked data/code, open-access documentation, end-to-end reproducible workflows, open-science resources, open-science tools, and a healthy community applying all the elements in their practice.

How to cite: Taposeea-Fisher, C., Smith, G., Dobrowolska, E., Giomo, D., Barchetta, F., Meißl, S., and Summers, D.: EarthCODE - a FAIR and Open Environment for collaborative research in Earth System Science , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7070, https://doi.org/10.5194/egusphere-egu25-7070, 2025.

EGU25-8114 | ECS | Orals | ESSI3.3

Flexible and scalable workflow framework HydroFlows for compound flood risk assessment and adaptation modelling 

Willem Tromp, Dirk Eilander, Hessel Winsemius, Tjalling De Jong, Brendan Dalmijn, Hans Gehrels, and Bjorn Backeberg

Flood risk assessments are increasingly guiding urban developments to safeguard against flooding. These assessments, consisting mainly of hazard and risk maps, make use of interconnected models consisting of a chain of climate, hydrological, hydraulic, and impact models, which are increasingly run interactively to support scenario modelling and decision-making in digital twins. To maintain interoperability, transparency, and reusability of this chain and the assessments themselves, using a workflow manager to manage the inter-model dependencies is a natural fit. However, composing and maintaining workflows is a non-trivial, time-consuming task, and they often have to be refactored for new workflow engines, or when changing compute environments, even if the workflow conceptually remains unchanged. These issues are particularly relevant in the development of digital twins for climate adaptation, where flood risk assessments serve as input to indicate high-risk areas. The complex model chain underpinning such digital twins can benefit greatly from transparent workflows that can be easily reused across different contexts.

To address these challenges, we developed the HydroFlows Python framework for composing and maintaining flood risk assessment workflows by leveraging common patterns identified across different workflows. The framework allows users to use one of the many steps available in the library or define workflow steps themselves and combine these into complete workflows which are validated on the fly. Available workflow steps include building, running, and postprocessing of models. Execution of the workflow is handled by one of the workflow managers to which our workflow description can be exported, such as Snakemake or tools with CWL support. This flexibility allows users to easily scale their workflows to different compute environments whenever the computational requirements demand so.

We demonstrate the flexibility of the HydroFlows framework by highlighting how it can be used to create complex workflows needed for digital twins supporting climate adaptation. HydroFlows not only enhances the flexibility and portability of the digital twin modelling workflows but also facilitates the integration of digital twin tooling and advanced computing and processing solutions to support interactive flood risk assessments in federated compute and data environments.

How to cite: Tromp, W., Eilander, D., Winsemius, H., De Jong, T., Dalmijn, B., Gehrels, H., and Backeberg, B.: Flexible and scalable workflow framework HydroFlows for compound flood risk assessment and adaptation modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8114, https://doi.org/10.5194/egusphere-egu25-8114, 2025.

EGU25-8305 | ECS | Posters on site | ESSI3.3

Enabling reliable workflow development with an advanced Testing Suite 

Alejandro Garcia Lopez, Leo Arriola Meikle, Gilbert Montane Pinto, Miguel Castrillo, Bruno de Paula Kinoshita, Eric Ferrer Escuin, and Aina Gaya Avila

Climate simulations require complex workflows that often integrate multiple components and different configurations per experiment, typically involving high-performance computing resources. The exhaustive testing required for these workflows can be time and resource consuming, presenting significant challenges in terms of computational cost and human effort. However, robust Continuous Integration (CI) testing ensures the reliability and reproducibility of such complex workflows by validating the codebase and ensuring the integrity of all the components used when performing climate simulations. Additionally, CI testing facilitates both major and minor releases, enhancing the efficiency of the development lifecycle.

To address these challenges, we present our Testing Suite software, designed to automate the setup, configuration, and execution of integration tests using Autosubmit, a workflow manager developed at the BSC. Autosubmit is typically used for climate modelling experiments, but also atmospheric composition ones, and also constitutes the backbone of some operational systems and Digital Twin initiatives. The Testing Suite software allows Autosubmit commands to be executed in batches and the responses from the Workflow Manager to be bypassed in a structured manner. By streamlining this process, it minimizes the effort required for exhaustive testing while ensuring reliability.

Beyond integration testing, the Testing Suite offers advanced capabilities for scientific result verification. By automatically comparing output data bit by bit, it swiftly detects regressions during test execution. Additionally, it provides CPMIP performance metrics, offering insights into the efficiency of the workflows.

As a result, the Testing Suite plays an important role in quality assurance, particularly during releases, where extensive testing ensures the workflow meets required functionality and performance standards across different configurations. These integration tests act as a checkpoint, validating the stability and robustness of the software before release. They also identify stable points in the main codebase, enabling developers to create new branches with confidence. This approach minimizes compatibility issues and facilitates a smoother development process.

In conclusion, the Testing Suite is a crucial part of the development lifecycle for climate simulations. It mitigates risks, ensures stability, and fosters innovation, all while maintaining a robust and reliable foundation for scientific research and development.

How to cite: Garcia Lopez, A., Arriola Meikle, L., Montane Pinto, G., Castrillo, M., de Paula Kinoshita, B., Ferrer Escuin, E., and Gaya Avila, A.: Enabling reliable workflow development with an advanced Testing Suite, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8305, https://doi.org/10.5194/egusphere-egu25-8305, 2025.

EGU25-8621 | ECS | Posters on site | ESSI3.3

Auto-EC-Earth: An automatic workflow to manage climate modelling experiments using Autosubmit 

Eric Ferrer, Gilbert Montane, Miguel Castrillo, and Alejandro Garcia

The European community Earth system model EC-Earth is based on different and interoperable climate components simulating different processes of the Earth system. This makes it a complex model that requires multiple input data sources for its various model components, which can be run in parallel with multiple configurations and resolutions, demanding different computational resources in each case.

The EC-Earth software contains a minimum set of scripts to manage the compilation and execution of the simulations, but these are not enough to perform all the tasks that experiments demand nor to guarantee the traceability and reproducibility of the entire workflow in a high-productivity scientific environment. For that matter, the Auto-EC-Earth software has been developed at the Earth Sciences department of the Barcelona Supercomputing Center (BSC-ES) relying on Autosubmit, a workflow manager also developed at BSC-ES.

We take advantage of the automatization provided by the workflow manager that allows us to configure, manage, orchestrate and share experiments with different configurations and target platforms. The workflow manager allows the user to split the run into different tasks that are executed on different local and remote machines, like the HPC platform where the simulation needs to be performed. This is achieved in a seamless integration between Autosubmit, the EC-Earth tools, and the different machines where the scripts run, all without any user-input required after the initial setup and the launch of the experiment thanks to the workflow developments. Autosubmit also allows to ensure traceability of the actual runs, to have all the required data available for different kinds of experiments separated and well documented.

However, running the main part of the simulation is a cooperative task between the Autosubmit workflow manager and the different tools used for each model version. Auto-EC-Earth workflow has evolved to adapt the best possible to the EC-Earth model scripts that are present to help with the model runs. In EC-Earth 4, ScriptEngine is used to manage the run, and it has been fully integrated into the Auto-EC-Earth 4 workflow and used to set up the environment, while Autosubmit still manages the submission of jobs to the HPC and the dependencies between them.

Auto-EC-Earth is a great example of a workflow system that has been developed and used throughout the years, well established within the BSC-ES and used in multiple production cases, like multiple CMIP exercises as well as a reference for newer ESM workflows like the one developed in the Destination Earth project. It has also allowed the BSC-ES to collaborate with the EC-Earth community through the testing of the new releases of the model.

How to cite: Ferrer, E., Montane, G., Castrillo, M., and Garcia, A.: Auto-EC-Earth: An automatic workflow to manage climate modelling experiments using Autosubmit, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8621, https://doi.org/10.5194/egusphere-egu25-8621, 2025.

EGU25-9175 | Posters on site | ESSI3.3

Enhancing Earth system models efficiency: Leveraging the Automatic Performance Profiling tool 

Roc Salvador Andreazini, Xavier Yepes Arbós, Stella Valentina Paronuzzi Ticco, Oriol Tintó Prims, and Mario Acosta Cobos

Earth system models (ESMs) are essential to understand and predict climate variability and change. However, their complexity and computational demands of high-resolution simulations often lead to performance bottlenecks that can impede research progress. Identifying and resolving these inefficiencies typically require significant expertise and manual effort, posing challenges for both climate scientists and High Performance Computing (HPC) engineers.

We propose automating performance profiling as a solution to help researchers concentrate on improving and optimizing their models without the complexities of manual profiling. The Automatic Performance Profiling (APP) tool brings this solution to life by streamlining the generation of detailed performance reports for climate models.

The tool ranges from high-level performance metrics, such as Simulated Years Per Day (SYPD), to low-level metrics, such as PAPI counters and MPI communication statistics. This dual-level reporting makes the tool accessible to a wide range of users, from climate scientists seeking a general understanding of the model efficiency, to HPC experts requiring granular insights for advanced optimizations.

Seamlessly integrated with Autosubmit, the workflow manager developed at the Barcelona Supercomputing Center (BSC), APP ensures compatibility with complex climate modelling workflows. By automating the collection and reporting of key metrics, APP reduces the effort and expertise needed for performance profiling, empowering users to enhance the scalability and efficiency of their climate models.

APP currently supports multiple models, including the EC-Earth4 climate model and the NEMO ocean model, and is compatible with different HPC systems, such as Marenostrum 5 and ECMWF’s supercomputer. Furthermore, the modular design of the tool allows adding new models and HPC platforms easily.

How to cite: Salvador Andreazini, R., Yepes Arbós, X., Paronuzzi Ticco, S. V., Tintó Prims, O., and Acosta Cobos, M.: Enhancing Earth system models efficiency: Leveraging the Automatic Performance Profiling tool, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9175, https://doi.org/10.5194/egusphere-egu25-9175, 2025.

Geo-simulation experiments (GSEs) are experiments allowing the simulation and exploration of Earth’s surface (such as hydrological, geomorphological, atmospheric, biological, and social processes and their interactions) with the usage of geo-analysis models (hereafter called ‘models’). Computational processes represent the steps in GSEs where researchers employ these models to analyze data by computer, encompassing a suite of actions carried out by researchers. These processes form the crux of GSEs, as GSEs are ultimately implemented through the execution of computational processes. Recent advancements in computer technology have facilitated sharing models online to promote resource accessibility and environmental dependency rebuilding, the lack of which are two fundamental barriers to reproduction. In particular, the trend of encapsulating models as web services online is gaining traction. While such service-oriented strategies aid in the reproduction of computational processes, they often ignore the association and interaction among researchers’ actions regarding the usage of sequential resources (model-service resources and data resources); documenting these actions can help clarify the exact order and details of resource usage. Inspired by these strategies, this study explores the organization of computational processes, which can be extracted with a collection of action nodes and related logical links (node-link ensembles). The action nodes are the abstraction of the interactions between participant entities and resource elements (i.e., model-service resource elements and data resource elements), while logical links represent the logical relationships between action nodes. In addition, the representation of actions, the formation of documentation, and the reimplementation of documentation are interconnected stages in this approach. Specifically, the accurate representation of actions facilitates the correct performance of these actions; therefore, the operation of actions can be documented in a standard way, which is crucial for the successful reproduction of computational processes based on standardized documentation. Aprototype system is designed to demonstrate the feasibility and practicality of the proposed approach. By employing this pragmatic approach, researchers can share their computational processes in a structured and open format, allowing peer scientists to re-execute operations with initial resources and reimplement the initial computational processes of GSEs via the open web.

How to cite: Zhu, Z. and Chen, M.: Reproducing computational processes in service-based geo-simulation experiments, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9791, https://doi.org/10.5194/egusphere-egu25-9791, 2025.

EGU25-10981 | Orals | ESSI3.3

yProv: a Software Ecosystem for Multi-level Provenance Management and Exploration in Climate Workflows 

Fabrizio Antonio, Gabriele Padovani, Ludovica Sacco, Carolina Sopranzetti, Marco Robol, Konstantinos Zefkilis, Nicola Marchioro, and Sandro Fiore

Scientific workflows and provenance are two faces of the same medal. While the former addresses the coordinated execution of multiple tasks over a set of computational resources, the latter relates to the historical record of data from its original sources. As experiments rapidly evolve towards complex end-to-end workflows, handling provenance at different levels of granularity and during the entire analytics workflow lifecycle is key for managing lineage information related to large-scale experiments in a flexible way as well as enabling reproducibility scenarios, thus playing a relevant role in Open Science.

The contribution highlights the importance of tracking multi-level provenance metadata in complex, AI-based scientific workflows as a way to foster documentation of data and experiments in a standardized format, strengthen interpretability, trustworthiness and authenticity of the results, facilitate performance diagnosis and troubleshooting activities, and advance provenance exploration. More specifically, the contribution introduces yProv, a joint research effort between CMCC and University of Trento targeting multi-level provenance management in complex, AI-based scientific workflows. The yProv project provides a rich software ecosystem consisting of a web service (yProv service) to store and manage provenance documents compliant with the W3C PROV family of standards, two libraries to track provenance in scientific workflows at different levels of granularity with a focus on AI models training (yProv4WFs and yProv4ML), and a data science tool for provenance inspection, navigation, visualization, and analysis (yProv Explorer). Activity on trustworthy provenance with yProv is also ongoing to fully address end-to-end provenance management requirements.

The contribution will cover the presentation of the yProv software ecosystem and use cases from the interTwin (https://www.intertwin.eu/) and ClimateEurope2 (https://climateurope2.eu/) European projects as well as from the ICSC National Center on HPC, Big Data and Quantum Computing targeting Digital Twins for extreme weather & climate events and data-driven/data-intensive workflows for climate change. 

How to cite: Antonio, F., Padovani, G., Sacco, L., Sopranzetti, C., Robol, M., Zefkilis, K., Marchioro, N., and Fiore, S.: yProv: a Software Ecosystem for Multi-level Provenance Management and Exploration in Climate Workflows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10981, https://doi.org/10.5194/egusphere-egu25-10981, 2025.

EGU25-11937 | Posters on site | ESSI3.3

DAM2 — A Scalable and Compliant Solution for Managing enriched Infrared images as FAIR Research Data  

Jean Dumoulin, Thibaud Toullier, Nathanael Gey, and Mathias Malandain

Abstract

Efficient and secure dataset management is a critical component of collaborative research projects, where diverse data types, sharing requirements, and compliance regulations converge. This work presents a dataset management tool entitled DAM2 (Data and Model Monitoring) developed within the Chips Joint Undertaking (Chips JU) funded European BRIGHTER project [1], to address these challenges. It provides a robust and adaptable solution for handling private and public ground based measurements datasets throughout the project lifecycle. These datasets combine infrared images (e.g. multispectral ones), with visible images, local weather measurements, labeled data, etc.

The tool is designed to ensure rights management, enabling selective data sharing among authorized partners based on predefined permissions. It incorporates secure access controls to safeguard sensitive data and meets GDPR (General Data Protection Regulation) requirements to guarantee compliance with European privacy standards. For public datasets, the tool integrates with Zenodo, an open-access repository, to support long-term storage and accessibility, aligning with the principles of open science. Key technical features include the usage of an open source, S3 compatible object storage server (MinIO [2]) providing scalability to manage large volumes of data. Additionally, the use of Zarr [3] data format behind the scene offers significant advantages for this cloud-based data management tool, including efficient storage of large datasets through chunking and compression, fast parallel read and write operations, and compatibility with a wide range of data analysis tools. The tool adheres to FAIR (Findable, Accessible, Interoperable, Reusable) principles, storing metadata alongside datasets to enhance usability and interoperability.

Developed as an open-source platform, the tool promotes transparency and collaboration while providing a complete and well-documented API for seamless integration with other systems. A user-friendly interface ensures accessibility for stakeholders with varying technical expertise, while the tool remains flexible to accommodate additional file formats as required. The development process incorporates insights from relevant COFREND (French Confederation for Non-Destructive Testing) working groups, to ensure alignment with broader initiatives in data management, interoperability and durability.

This paper addresses the design, study and developed platform. First operational functionalities are demonstrated through the manipulation of first BRIGHTER and other research project datasets.

In conclusion, DAM2 is a comprehensive solution for managing diverse datasets in collaborative projects, balancing security, compliance, and accessibility. It provides a foundation for efficient, compliant, and interoperable data handling while supporting the principles of open science and FAIR data management.

Perspectives include expanding interoperability with additional repositories, incorporating advanced analytic and visualization features, and integrating AI-driven automation.

Acknowledgments

Authors would like to acknowledge the BRIGHTER HORIZON project. BRIGHTER has received funding from the Chips Joint Undertaking (JU) under grant agreement No 101096985. The JU receives support from the European Union’s Horizon Europe research and innovation program and France, Belgium, Portugal, Spain, Turkey.

References

[1] Brighter --- Project-Brighter. https://project-brighter.eu/, accessed on January 2025.

[2] MinIO, Inc. MinIO S3 Compatible Storage for AI --- Min.Io. https://min.io/, accessed on January, 2025.

[3] Zarr --- Zarr.dev. https://zarr.dev/, accessed on January, 2025.

How to cite: Dumoulin, J., Toullier, T., Gey, N., and Malandain, M.: DAM2 — A Scalable and Compliant Solution for Managing enriched Infrared images as FAIR Research Data , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11937, https://doi.org/10.5194/egusphere-egu25-11937, 2025.

EGU25-13604 | ECS | Orals | ESSI3.3

Streamlining configurations of process-based models through extensible and free workflows 

Kasra Keshavarz, Alain Pietroniro, Darri Eythorsson, Mohamed Ismaiel Ahmed, Paul Coderre, Wouter Knoben, Martyn Clark, and Shervan Gharari

High-resolution and high-complexity process-based hydrological models play a pivotal role in advancing our understanding and prediction of water cycle dynamics, particularly in ungauged basins and under nonstationary climate conditions. However, the configuration, application, and evaluation of these models are often hindered by the intricate and inconsistent nature of a priori information available in various datasets, necessitating extensive preprocessing steps. These challenges can limit the reproducibility, applicability, and accessibility of such models for the broader scientific user community. To address these challenges, we introduce our generalized Model-Agnostic Framework (MAF), aimed at simplifying the configuration and application of data-intensive process-based hydrological models. Through a systematic investigation of commonly used models and their configuration procedures, we provide workflows designed to streamline the setup process for this category of hydrological models. Building on earlier efforts, this framework adheres to the principle of separating model-agnostic and model-specific tasks in the setup procedure of such models. The model-agnostic workflows focus on both dynamic datasets (e.g., meteorological data) and static datasets (e.g., land-use maps), while the model-specific components feed preprocessed, relevant data to the hydrological models of interest. Our initial prototypes of MAF includes recipes for various static and dynamic datasets and also tailored model-specific workflows for MESH, SUMMA, and HYPE process-based modelling frameworks. We demonstrate the effectiveness of these novel workflows in reducing configuration complexity and enhancing the reproducibility of process-based hydrological models through test applications in high-performance computing environments. The framework automates numerous manual tasks, significantly saving time, and enabling continuity in research efforts. Moreover, by minimizing human error and enhancing reproducibility, this research has fostered collaboration with several Canadian government entities, leveraging sophisticated process-based models to address complex environmental challenges.

How to cite: Keshavarz, K., Pietroniro, A., Eythorsson, D., Ahmed, M. I., Coderre, P., Knoben, W., Clark, M., and Gharari, S.: Streamlining configurations of process-based models through extensible and free workflows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13604, https://doi.org/10.5194/egusphere-egu25-13604, 2025.

EGU25-18040 | ECS | Posters on site | ESSI3.3

Workflows for numerical reproducibility in the OceanVar data assimilation model 

Francesco Carere, Francesca Mele, Italo Epicoco, Mario Adani, Paolo Oddo, Eric Jansen, Andrea Cipollone, and Ali Aydogdu

Numerical reproducibility is a crucial yet often overlooked challenge in ensuring the credibility of computational results and the validity of Earth system models. In large-scale, massively parallel simulations, achieving numerical reproducibility is complicated by factors such as heterogeneous HPC architectures, floating point intricacies, complex hardware/software dependencies, and the non-deterministic nature of parallel execution.

This work addresses the challenges of debugging and ensuring bitwise reproducibility (BR) in parallel simulations, specifically for the MPI-parallelised OceanVar data assimilation model. We explore methods for detecting and resolving BR-related bugs, focusing on an automated debugging process. Currently mature tools to automate this process are lacking for bugs due to MPI-parallelisation, making automatic BR verification in scientific workflows involving such codebases a time-consuming challenge.

However, BR is sometimes considered unrealistic in workflows involving heterogeneous computing architectures. As an alternative, statistical reproducibility (SR) is proposed and explored by various research groups in the Earth system modelling community, for which automated tools have been developed. For example, the scientific workflow of CESM supports automatic verification of SR using the CESM-ECT framework/PyCECT software. In case of failure of SR a root-cause analysis tool exists, CESM-RUANDA, albeit currently not fully functional. We explore SR as an alternative and complementary approach to of BR focusing on its potential to support numerical reproducibility in workflows involving heterogeneous computing architectures.

How to cite: Carere, F., Mele, F., Epicoco, I., Adani, M., Oddo, P., Jansen, E., Cipollone, A., and Aydogdu, A.: Workflows for numerical reproducibility in the OceanVar data assimilation model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18040, https://doi.org/10.5194/egusphere-egu25-18040, 2025.

EGU25-18890 | Posters on site | ESSI3.3

Research data management for numerical simulations in Earth-System Science 

Klaus Getzlaff and Markus Scheinert

One of today's challenges is the effective access to scientific data either within research groups or across different institutions to increase the reusability of the data and therefore their value. While large operational modeling and service centers have enabled query and access to data via common web services, this is often not the case for smaller institutions or individual research groups. Especially the maintenance of the infrastructure and the simplicity of the workflows, in order to make the data and their provenance available and accessible, are common challenges for scientists and data management.

At GEOMAR there are several data steward positions to support RDM for special disciplines and formats. They are also connected across centres to work on common standards, e.g. the netcdf standard working group in the Helmholtz Earth and Environment DataHUB.

Here we will present the institutional approach on research data management for numerical simulations in earth system science. The data handling, especially the possibilities for data sharing, publication and access, which is in today’s focus, is realized by using persistent identifier handles in combinations with a modern http web server index solution and a THREDDS server allowing remote access using standardized protocols such as OPeNDAP, WMS. By cross-linking this into the central institutional metadata and publication repositories it allows the re-usability of the data by scientists from different research groups and backgrounds. In addition to the pure data handling the documentation of the numerical simulation experiments is of similar importance to allow re-usability or reproducibility and to provide the data which will be addressed too.

How to cite: Getzlaff, K. and Scheinert, M.: Research data management for numerical simulations in Earth-System Science, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18890, https://doi.org/10.5194/egusphere-egu25-18890, 2025.

EGU25-19655 | Posters on site | ESSI3.3

Multi-faceted habitat connectivity: how to orchestrate remote sensing with citizen science data? 

Ivette Serral, Vitalii Kriukov, Lucy Bastin, Riyad Rahman, and Joan Masó

In the era of declining biodiversity, global climate change and transformations in land use, terrestrial habitat connectivity is one of the key parameters of ecosystem management. In this regard, the land-use/land-cover (LULC) dynamics is crucial to detect the spatiotemporal trends in connectivity of focal endangered species and to predict the effects for biodiversity for planned or proposed LULC changes.

Apart from the LULC derivatives of remote sensing, connectivity analysis and scenarios modelling can also benefit from citizen science datasets, such as Open Street Map and GBIF species occurrence data cubes in which aggregated data can be perceived as a cube with three dimensions - taxonomic, temporal and geographic. The synthetic LULC datasets which cover Catalonia every 5 years (1987-2022) were enriched via developed Data4Land harmonisation tool harnessing Open Street Map (through Overpass Turbo API) and World Database on Protected Areas. Two outstanding well-known tools, Graphab and MiraMon GIS&RS (using the Terrestrial Connectivity Index Module - ICT), were used to create the overarching dataset on terrestrial habitat connectivity in Catalonia (2012-2022) for target species and broad land cover categories, forests. Significant decline trends in forest habitat connectivity are observed for Barcelona metropolitan area, and vice versa in the Pyrenees mountain corridor and protected areas. According to the local case study on the connectivity of Mediterranean turtle in the Albera Natural Park, general positive trend was affected by massive fires in 2012.

To ensure the replicable results, the pipeline to create reliable metadata in accordance with FAIR principles, especially data lineage, is being developed, as well as the high performance computing pipeline for Graphab.

How to cite: Serral, I., Kriukov, V., Bastin, L., Rahman, R., and Masó, J.: Multi-faceted habitat connectivity: how to orchestrate remote sensing with citizen science data?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19655, https://doi.org/10.5194/egusphere-egu25-19655, 2025.

EGU25-21553 | Posters on site | ESSI3.3

European Digital Twin of the Ocean: the integration with EuroHPC platforms 

Stella Valentina Paronuzzi Ticco, Simon Lyobard, Mathis Bertin, Quentin Gaudel, Jérôme Gasperi, and Alain Arnaud

The EDITO platform serves as the foundational framework for building the European Digital Twin of the Ocean, seamlessly integrating oceanographic data, processes and services on a single and comprehensive platform. The platform provides scalable computing resources interconnected with EuroHPC supercomputing centers. We have developed a mechanism that allows users to remotely execute functions (processes) on HPCs and store the resulting output at the location of their choice (e.g. EDITO personal storage, third parties S3 buckets, etc.). This output can then be leveraged as input for subsequent processes, fostering a streamlined and interconnected workflow. Our presentation will delve into the technical details to achieve such an integration between cloud and HPC systems. 

How to cite: Paronuzzi Ticco, S. V., Lyobard, S., Bertin, M., Gaudel, Q., Gasperi, J., and Arnaud, A.: European Digital Twin of the Ocean: the integration with EuroHPC platforms, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21553, https://doi.org/10.5194/egusphere-egu25-21553, 2025.

NP5 – Predictability

EGU25-872 | ECS | Posters on site | CL4.8

A new orographic drag parameterization package for the GLOBO model: implementation and evaluation  

Guido Davoli, Daniele Mastrangelo, Annalisa Cherchi, and Andrea Alessandri

Orography plays a fundamental role in shaping the atmospheric circulation and affects key atmospheric processes. Therefore, weather and climate models must adequately represent its effects to obtain accurate predictions. Since all orographic scales are found to influence the atmospheric flow, the parameterization of unresolved orographic drag has been recognized as crucial to simulate a realistic mid-latitude circulation. Moreover, in the last few years, it has become clear that orographic gravity wave drag (OGWD) and turbulent orographic form drag (TOFD) parameterization schemes play a crucial role in reducing some of the long-standing circulation biases affecting climate models. However, they are still considered a potential source of errors, due to the uncertainties which affect some poorly constrained physical parameters. Furthermore, these schemes need boundary conditions suitable to characterize the physical features of sub-grid orography. The strategies for the generation of such boundary conditions can vary a lot between different modelling centres, and it has been shown to be an important source of uncertainty. 

GLOBO is a global atmospheric general circulation model developed at the Institute for Atmospheric Science and Climate of the Italian National Research Council (ISAC-CNR). It is currently in use within many operational frameworks, including a global monthly probabilistic forecast system that contributes to the Subseasonal-to-seasonal (S2S) project database. In an effort to improve and modernize the model, we implemented a novel orographic drag parameterization package, based on state-of-the-art OGWD and TOFD schemes. Simultaneously with the development of the orographic drag parameterizations, we developed a novel software package, OROGLOBO (OROGraphic ancillary files generator for GLOBal atmospheric mOdels) designed for the generation of the orographic boundary conditions. This unique open-source tool is designed to exploit a state-of-the-art, high resolution global Digital Elevation Model to generate boundary conditions for OGWD and TOFD schemes, gathering the main algorithms and techniques available in the literature in a single software. 

Here, we present the results of this model update. A new set of retrospective forecasts was performed, consisting of an 8-members ensemble, initialized every 5 days and integrated for 35 days, during the period 2001-2020, including the developments in orographic physical parameterization and boundary conditions. This set of simulations is compared to the corresponding hindcasts set performed with the standard model configuration and used to calibrate the operational ensemble of global sub-seasonal probabilistic forecasts. We evaluate the impact of the improved representation of unresolved orographic drag on the simulation and prediction of the Northern Hemisphere mid-latitudes circulation. We assess the change in prediction skill for atmospheric blocking events and associated extreme temperature and wind conditions. 

How to cite: Davoli, G., Mastrangelo, D., Cherchi, A., and Alessandri, A.: A new orographic drag parameterization package for the GLOBO model: implementation and evaluation , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-872, https://doi.org/10.5194/egusphere-egu25-872, 2025.

EGU25-1040 | ECS | Orals | CL4.8

Understanding Soil Modulation of Drought Persistence in CMIP6 Models 

Marco Possega, Emanuele Di Carlo, Vincenzo Senigalliesi, and Andrea Alessandri

 Drought persistence is a critical factor in assessing water availability and its impacts on agriculture, ecosystems, and society. In this respect, poorly constrained soil properties in climate models such as field capacity – i.e. the maximum water a soil can retain after drainage of excess moisture – may strongly affect severity and persistence of simulated soil drought conditions. This study examines for the first time the regulating role of soil properties, particularly of field capacity, in shaping drought memory and its broader impacts. Using the CMIP6 multi-model ensemble and observations, we analyze drought dynamics across various phases of the hydrological cycle applying non-parametric standardized indices: Standardized Precipitation Index (precipitation deficits), Standardized Precipitation-Evapotranspiration Index (precipitation-evapotranspiration balance), Standardized Soil Moisture Index (soil moisture deficits), and Standardized Runoff Index (reduced runoff). Our analysis investigates the persistence between hydrological drought indicators, showing that soils with greater field capacity sustain drought conditions longer, emphasizing the importance of accurately modeling soil properties to capture drought persistence effectively. The historical CMIP6 simulations are compared with observational datasets, including GLEAM and CRU, to assess the deviation between model outputs and observed climate conditions. The future scenarios (SSP126, SSP245, SSP370, SSP585) are also examined, revealing significant regional differences in projected drought behavior depending on the degree of radiative-forcing increase during 21st century. High-emission scenarios project prolonged drought conditions due to increased temperatures and evapotranspiration feedback, while low-emission pathways are effective in preserving more stable hydrological dynamics. Our results show that, in water limited and transition areas such as the Euro-Mediterranean region, the persistence of droughts and its projected change considerably depend on the modeled field capacity. This study highlights the essential role of field capacity and other soil characteristics in regulating the variability and the persistence of drought events. By bridging historical validation with future projections, it provides a comprehensive understanding of drought dynamics and trends, also identifying observational constraints for the Earth System Models. These findings are crucial for refining predictions of agricultural and hydrological drought impacts and for guiding adaptation strategies in water-limited regions that are vulnerable to drought exacerbation under climate change.

How to cite: Possega, M., Di Carlo, E., Senigalliesi, V., and Alessandri, A.: Understanding Soil Modulation of Drought Persistence in CMIP6 Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1040, https://doi.org/10.5194/egusphere-egu25-1040, 2025.

EGU25-1545 | Posters on site | CL4.8

Sub-seasonal to Seasonal Arctic Summer Sea Ice Forecasts Using Dynamical Downscaling with the Regional Arctic System Model 

Younjoo Lee, Wieslaw Maslowski, Anthony Craig, Jaclyn Clement Kinney, and Robert Osinski

The Arctic region has been warming at a rate significantly faster than the global average, leading to an accelerated decline in sea ice. This trend is expected to continue, potentially resulting in a "low-ice regime," which could make sea ice conditions more unpredictable. Anticipating changes in Arctic sea ice and climate states is therefore crucial for guiding various human activities, from natural resource management to risk assessment decisions. While global climate and Earth system models project continuous sea ice decline over decadal time scales, achieving reliable seasonal forecasts remains challenging. To address this, we apply dynamical downscaling with the state-of-the-art Regional Arctic System Model (RASM), which enables us to forecast Arctic sea ice on time scales ranging from weeks to six months. RASM is a fully coupled regional climate model that integrates components for the atmosphere, ocean, sea ice, and land, interconnected through the flux coupler of the Community Earth System Model. In our study, we simulate RASM at a horizontal resolution of 1/12 degree (approximately 9 km) for both the ocean and sea ice, with 45 vertical levels in the ocean and five thickness categories for sea ice. The atmosphere is configured on a 50-km grid with 40 vertical levels, dynamically downscaled from the NOAA/NCEP Climate Forecasting System version 2 (CFSv2) at 72-hour intervals for the upper half of the atmosphere. Monthly ensemble forecasts extending up to six months are generated using initial conditions derived from a fully-coupled RASM hindcast simulation without bias correction and assimilation. This presentation highlights results for September sea ice predictions initialized on April 1, May 1, June 1, July 1, August 1, and September 1, covering pan-Arctic and regional sea ice spatio-temporal conditions from 2012 to 2021. Specifically, we examine how lead time and initial conditions affect the quantitative skill of seasonal predictability for Arctic sea ice and demonstrate skillful predictions of September sea ice up to six months in advance. Overall, our study underscores that enhancing model physics and obtaining more realistic initial conditions are crucial for achieving skillful sub-seasonal to seasonal predictions.

How to cite: Lee, Y., Maslowski, W., Craig, A., Clement Kinney, J., and Osinski, R.: Sub-seasonal to Seasonal Arctic Summer Sea Ice Forecasts Using Dynamical Downscaling with the Regional Arctic System Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1545, https://doi.org/10.5194/egusphere-egu25-1545, 2025.

EGU25-1847 | Orals | CL4.8

AI deep learning for climate forecasts 

Jing-Jia Luo

AI deep learning for climate science has attracted increasing attentions in recent years with rapidly expanded applications to many areas. In this talk, I will briefly present our recent progresses on using various deep learning methods for seasonal-to-multi-seasonal predictions of ENSO, the Indian Ocean Dipole (IOD), summer precipitation in China and East Africa, Arctic sea ice cover, ocean waves, as well as the bias correction and downscaling of dynamical model’s forecasts. The results suggest that many popular deep learning methods, such as convolutional neural networks, residual neural network, long-short term memory, ConvLSTM, multi-task learning, cycle-consistent generative adversarial networks and vision transformer, can be well applied to improve our understanding and predictions of climate. In addition, a brief introduction of AI large models for ensemble weather-subseasonal-seasonal-decadal forecasts, together with the perspective on the future development of AI methods, will also be presented.

How to cite: Luo, J.-J.: AI deep learning for climate forecasts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1847, https://doi.org/10.5194/egusphere-egu25-1847, 2025.

EGU25-2210 | ECS | Posters on site | CL4.8

The role of Pacific Tropical Instability Wave in Sub-Seasonal SST predictability  

Li Tianyan, Yu Yongqiang, and Zhen Weipeng

Tropical Instability Waves (TIWs) play a crucial role in modulating Sea Surface Temperature (SST) variability in tropical oceans, yet their representation in current forecast systems remains challenging. This study investigates the relationship between TIWs and sub-seasonal SST predictability while evaluating the performance limitations of the Licoms Forecast System. Through comprehensive analysis of observational data and model outputs, we demonstrate that TIWs provide significant potential for enhancing sub-seasonal SST forecast skill through their regular wave patterns and predictable evolution characteristics. However, our findings reveal that the current Licoms forecast systems systematically underestimate both TIW intensity and wavelength. Critical examination of error sources indicates that these deficiencies primarily originate from initialization fields rather than model physics or dynamics. 

How to cite: Tianyan, L., Yongqiang, Y., and Weipeng, Z.: The role of Pacific Tropical Instability Wave in Sub-Seasonal SST predictability , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2210, https://doi.org/10.5194/egusphere-egu25-2210, 2025.

EGU25-3974 | Orals | CL4.8

Increased multi-year ENSO predictability under greenhouse gas warming accounted by large ensemble simulations and deep learning 

Young-Min Yang, Jae-Heung Park, June-Yi Lee, Soon-Il An, Sang-Wook Yeh, Jong-Seoung Kug, and Yoo-Geun Ham

The El Niño/Southern Oscillation (ENSO) is the primary internal climatic driver shaping extreme events worldwide1,2,3. Its intensity and frequency in response to greenhouse gas (GHG) warming has puzzled scientists for years, despite consensus among models about changes in average conditions4-16. Recent research has shed light on changes not only in ENSO variability5,7,8,10,13, but also in the occurrence of extreme5,6,11,12,13,14 and multi-year El Niño4,15, and La Niña9,11,16 events under GHG warming. Here, we investigate potential changes in ENSO predictability associated with changes in ENSO dynamics in the future by using long-range deep-learning forecasts trained on extensive large ensemble simulations of Earth System Models under historical forcings and the future high GHG emissions scenario. Our results show a remarkable increase in the predictability of ENSO events, ranging from 35% to 65% under the high GHG emissions scenario due to reduced ENSO irregularity, supported by a broad consensus among multi-models. Under GHG warming, an El Nino-like warming flattens the thermocline depth with upper ocean stratification. This flattening of the thermocline depth leads to an increased transition frequency between El Niño and La Niña events, driven by strengthened recharge-discharge oscillation with enhanced thermocline feedback and SST responses to zonal wind stress. As a result, ENSO complexity would reduce with increased regularity and reduced skewness, increasing ENSO predictability. These results imply that the future social and economic impacts of ENSO events may be more manageable, despite an expected increase in the frequency of extreme ENSO events.

How to cite: Yang, Y.-M., Park, J.-H., Lee, J.-Y., An, S.-I., Yeh, S.-W., Kug, J.-S., and Ham, Y.-G.: Increased multi-year ENSO predictability under greenhouse gas warming accounted by large ensemble simulations and deep learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3974, https://doi.org/10.5194/egusphere-egu25-3974, 2025.

EGU25-5233 | Orals | CL4.8

Standardisation of equitable climate services by supporting a community of practice 

Francisco Doblas-Reyes, Asun Lera St Clair, Marina Baldissera Pacchetti, Paula Checchia, Joerg Cortekar, Judith E.M. Klostermann, Werner Krauß, Angel Muñoz, Jaroslav Mysiak, Jorge Paz, Marta Terrado, Andreas Villwock, Mirjana Volarev, and Saioa Zorita

Climate services are essential to support climate-sensitive decision making, enabling adaptation to climate change and variability, and mitigate the sources of anthropogenic climate change, while considering the values and contexts of those involved. The unregulated nature of climate services can lead to low market performance and lack of quality assurance. Best practices, guidance, and standards serve as a form of governance, ensuring quality, legitimacy, and relevance of climate services. The Climateurope2 project (www.climateurope2.eu) addresses this gap by engaging and supporting an equitable and diverse community of climate services to provide recommendations for their standardisation. Four components of climate services are identified (the decision context, the ecosystem of actors and co-production processes, the multiple knowledge systems involved, and the delivery and evaluation of these services) to facilitate analysis. This has resulted in the identification of nine key messages summarising the susceptibility for the climate services standardisation. The recommendations are shared with relevant standardisation bodies and actors as well as with climate services stakeholders and providers.

How to cite: Doblas-Reyes, F., Lera St Clair, A., Baldissera Pacchetti, M., Checchia, P., Cortekar, J., Klostermann, J. E. M., Krauß, W., Muñoz, A., Mysiak, J., Paz, J., Terrado, M., Villwock, A., Volarev, M., and Zorita, S.: Standardisation of equitable climate services by supporting a community of practice, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5233, https://doi.org/10.5194/egusphere-egu25-5233, 2025.

EGU25-7271 | ECS | Posters on site | CL4.8

Impact-Based Forecasting Model for Flood Hazard Mitigation in Java, Indonesia 

Dendi Rona Purnama, Simon F. B. Tett, Ruth Doherty, and Ida Pramuwardani

Flooding is the most frequent and damaging hydrometeorological disaster in Indonesia, with Java being especially vulnerable due to its dense population and rapid urbanization. This study aims to refine the Impact-Based Forecasting (IBF) model to improve flood hazard predictions and mitigation efforts. Using Global Precipitation Measurement (GPM-IMERG) rainfall data as the hazard component combined with vulnerability and capacity datasets from InaRISK, this research focuses on enhancing the precision and reliability of impact assessments.

Initial analyses highlight the potential of impact-based rainfall thresholds and assessment probabilistic impacts to refine the IBF model and reduce subjectivity in impact assessments. By linking calculated impact values and disaster magnitudes for the 2014 – 2023 period, this study shows a promising skill for significant and severe flood events, although improvements are needed for minor and minimal disaster classifications.

This research lays the groundwork for a more robust and scalable IBF model tailored to Java’s unique challenges. The findings aim to support BMKG’s operational needs, enabling the delivery of more actionable early warnings and targeted disaster preparedness measures. By addressing critical gaps in existing IBF systems, this study contributes to bridging the divide between hazard-impact forecasts and societal resilience, ultimately mitigating the impacts of floods in Indonesia.

How to cite: Purnama, D. R., Tett, S. F. B., Doherty, R., and Pramuwardani, I.: Impact-Based Forecasting Model for Flood Hazard Mitigation in Java, Indonesia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7271, https://doi.org/10.5194/egusphere-egu25-7271, 2025.

EGU25-9933 | Orals | CL4.8

Hydroclimate services are more than just providing data 

Jean-Philippe Vidal, Eric Sauquet, Louis Héraut, Sonia Siauve, Guillaume Evin, Jean-Michel Soubeyroux, Flore Tocquer, Audrey Bornançin-Plantier, Claire Magand, and Maud Berel

The concept of hydroclimate services is predominantly recognised as web portals dedicated to the dissemination of data to potential users. However, the scope of climate services extends beyond the sole provision of data. This communication presents a comprehensive ecosystem of tools and resources associated with the development of an updated national hydrological projection dataset in France. The ecosystem was brought to life through a close collaboration between scientists and water managers in two joint projects: Explore2 and LIFE Eau&Climat. Tools and resources were thus developped with and for water resource managers, and designed to enhance the comprehension of both the conceptual framework and the data itself, facilitating utilisation in accordance with best practices for climate change adaptation.

The project websites serve as gateways to the ecosystem and the tools: the Explore2 website contains interviews with the scientific contributors, and the LIFE Eau&Climat website is hosted by the national website dedicated to water managers. A summary of the joint final public event accompanies the replay of the one-day conference and debates on a dedicated website. A compendium of antecedent research projects on climate change impacts on hydrology has been collated to summarise the state of the art prior to the two projects. A MOOC has been developed in conjunction with scientists to facilitate the comprehension of the Explore2 project, its design, and its application in adaptation studies.

Moreover, the Explore2 dataverse (https://entrepot.recherche.data.gouv.fr/dataverse/explore2) brings together a variety of products in an organised and searchable way, including thematic scientific reports, GIS layers, and other key metadata. It also contains three types of station datasheets aimed at locally contextualising outputs: hydrological model performance datasheets, projection results datasheets, and uncertainty quantification datasheets. The MEANDRE interactive data visualisation tool (https://meandre.explore2.inrae.fr/) offers a guided tour of the salient take-home messages and a comprehensive exploration of the Explore2 hydrological projection dataset. This multi-model dataset (GCMs/RCMs/bias correction methods/hydrological models) is made available through the DRIAS-Eau portal (https://drias-eau.fr/), which functions as a water mirror of the established DRIAS-Climat portal. The utilisation of this dataset for local climate change impact studies is facilitated by a methodological guide written as an adventure gamebook (https://livreec.inrae.fr/) and based on real-life studies carried out by water managers during the LIFE Eau&Climat project. Furthermore, experiments of sonification of hydrological projections offer a novel approach to apprehending future changes (https://explore2enmusique.github.io/).

This ecosystem has been met with great anticipation and acclaim by local to national-scale water managers, paving the way for ongoing local prospective studies. These will be able to confront future resources with the ecological needs of aquatic environments and human water usage.

This work is funded by the EU LIFE Eau&Climat project (LIFE19 GIC/FR/001259).

How to cite: Vidal, J.-P., Sauquet, E., Héraut, L., Siauve, S., Evin, G., Soubeyroux, J.-M., Tocquer, F., Bornançin-Plantier, A., Magand, C., and Berel, M.: Hydroclimate services are more than just providing data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9933, https://doi.org/10.5194/egusphere-egu25-9933, 2025.

EGU25-11600 | ECS | Orals | CL4.8

Windows of Opportunity for Seasonal Prediction of droughts: the case of the Middle East 

Thomas Dal Monte, Andrea Alessandri, Annalisa Cherchi, Markus Donat, and Marco Gaetani

Drought warnings are vital to sectors like agriculture and water management, especially at the seasonal time scale. Identifying the sources of drought predictability in regions where a prediction system demonstrated potential for useful applications of the forecasts, represents an important step toward building confidence in the predictions and refining the seasonal predictions. To better identify higher forecast skill in this context, one possible approach is to focus on specific “windows of opportunity”. The approach aims to identify periods when persistent anomalies occurring in the ocean, the atmosphere or the land surface may positively precondition the predictive ability of the seasonal forecast. In the case of SPI3, a high potential for preconditioned predictive skill is identified in the Middle East region, as suggested by a robust relationship with large-scale climate modes. Building on these results, this study explores the contributions of individual years to the skill for the region during the autumn season and in the hindcast period 1993-2016. We used a Multi Model Ensemble (MME) of eight seasonal prediction systems (SPSs) provided by the Copernicus Climate Data Store (CDS) and observations from the Climate Research Unit (CRU) to calculate the SPI3 time series and the values of the Pacific and Indian teleconnection indices, the Oceanic Nino Index (ONI) and the Dipole Mode Index (DMI), respectively. A novel methodology is implemented to cluster the year-by-year MME contributions to the Pearson correlation coefficient (PCC) that are preconditioned by the large-scale teleconnections. 

Results indicate that years with extreme high or low values of ONI and DMI are the main contributors to the forecasting skill of the MME drought predictions over the Middle East. In particular, a window of opportunity is identified in four (out of 24) years that show significantly high contribution to overall skill. These years are robustly preconditioned by El Niño or La Niña events. Among the years with higher contributions, 1994 stands out as being more influenced by the DMI, thus driven primarily by SST anomalies in the Indian Ocean rather than the Pacific Ocean.  The methodological approach developed in this study successfully highlighted the potential windows of opportunity for seasonal prediction in the Middle East region, and could be applied extensively to develop early warnings for the coming seasons to serve agriculture and water management operations.

How to cite: Dal Monte, T., Alessandri, A., Cherchi, A., Donat, M., and Gaetani, M.: Windows of Opportunity for Seasonal Prediction of droughts: the case of the Middle East, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11600, https://doi.org/10.5194/egusphere-egu25-11600, 2025.

EGU25-11821 | Orals | CL4.8

Seamless seasonal to multi-annual climate predictions by constraining transient (CMIP6) climate model simulations 

Juan C. Acosta Navarro, Alvise Aranyossy, Paolo De Luca, Markus G. Donat, Arthur Hrast Essenfelder, Rashed Mahmood, Andrea Toreti, and Danila Volpi

Seamless climate predictions combine information across different timescales to deliver information potentially useful for sectors like agriculture, energy, and public health. Seamless operational forecasts for periods spanning from sub-annual to multi-annual timescales are currently not available throughout the year. We show that this gap can be closed by using a well-established climate model analog method. The method consists in sampling model states from the CMIP6 transient simulation catalog based on their similarity with the observed sea surface temperature as a means of model initialization. 

Here we present the methodology and basic skill evaluation of the analog-based temperature and standardized precipitation index retrospective predictions with forecast times ranging from 3 months up to 4 years. We additionally compare these predictions with the non-initialized CMIP6 ensemble and with two operational benchmarks produced with state-of-the-art dynamical forecasts systems: one on seasonal timescales and the other on annual to multi-annual timescales.

The analog method provides skillful climate predictions across the different timescales, from seasons to several years, offering temperature and precipitation forecasts comparable to those from state-of-the-art initialized climate prediction systems, particularly at the annual to multi-annual timescales. However, unlike operational decadal prediction systems that provide only one or two initializations per year, the analog-based system can generate seamless predictions with monthly initializations, offering year-round climate information. Additionally, analog predictions are computationally inexpensive once the multi-model transient climate simulations have been completed. We argue that these predictions are a valuable complement to existing operational prediction systems and may improve regional climate adaptation and mitigation strategies. 

 

How to cite: Acosta Navarro, J. C., Aranyossy, A., De Luca, P., Donat, M. G., Hrast Essenfelder, A., Mahmood, R., Toreti, A., and Volpi, D.: Seamless seasonal to multi-annual climate predictions by constraining transient (CMIP6) climate model simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11821, https://doi.org/10.5194/egusphere-egu25-11821, 2025.

EGU25-13385 | Posters on site | CL4.8

Representation of Temporal Variations of Vegetation in Reanalysis and Climate Predictions: Diverging Soil-Moisture Response in Land Surface Models 

Andrea Alessandri, Marco Possega, Emanuele Di Carlo, Annalisa Cherchi, Souhail Boussetta, Gianpaolo Balsamo, Constantin Ardilouze, Gildas Dayon, and Fransje van Oorschot

Vegetation plays a crucial role in the land surface water and energy balance modulating the interactions and feedback with climate at the regional to global scale. The availability of unprecedented Earth observation products covering recent decades (and extended up to real-time) are therefore of paramount importance to better represent the vegetation and its time evolution in the land surface models (LSMs) used for offline analysis/initialization and for the seasonal-to-decadal predictions. 

Here, we integrate realistic vegetation Leaf Area Index (LAI) variability from latest generation satellite campaigns, available through Copernicus Land Monitoring Service (CLMS), in three different LSMs that conducted the same coordinated set of offline land-only simulations forced by hourly atmospheric fields derived from the ERA5 atmospheric reanalysis. The experiment implementing realistic interannually-varying LAI (SENS) is compared with simulations utilizing a climatological LAI (CTRL) to quantify the vegetation feedback and the effects on the simulation of near-surface soil moisture.

The results show that the inter-annually varying LAI considerably affects the simulation of near-surface soil moisture anomalies in all three models and over the same water-limited regions, but surprisingly the effects diverge among models: compared with ESA-CCI observations, the near-surface soil moisture anomalies significantly improve in  one of the three LSMs (HTESSEL-LPJGuess) while the other two (ECLand and ISBA-CTRIP) display opposite effects with significant worsening of the anomaly correlation coefficients. It is found that the enhanced simulation of near-surface soil moisture is enabled by the positive feedback that is activated by the effective vegetation cover (EVC) parameterization, implemented only in HTESSEL-LPJGuess. The EVC parameterization works such that the effective fraction of the bare soil being covered by vegetation does vary with LAI following an exponential function constrained by available satellite observations. The increased (reduced) soil-moisture limitation during dry (wet) periods produces negative (positive) LAI and therefore EVC anomalies, which in turn generate a dominating positive feedback on the near-surface soil moisture of HTESSEL-LPJGuess by exposing more (less) bare soil to direct evaporation from the sub-surface layer. On the other hand, in the EC-Land and ISBA-CTRIP models, EVC is fixed in time as it cannot vary with LAI and so the positive feedback described cannot be activated. The only feedback on near-surface soil moisture anomalies that operates  in these two models is negative and comes from the reduced (increased) transpiration related to the negative (positive) LAI anomalies.

Simply prescribing observed vegetation data into LSMs does not guarantee the introduction of the correct coupling and feedback on climate. In this respect, this multi-model comparison experiment demonstrates the fundamental role of the inclusion of the underlying vegetation processes in LSMs. Ignoring the proper representation of the vegetation processes could lead to unrealistic (and even the opposite effects compared with observations) behaviour in reanalysis and climate predictions.

How to cite: Alessandri, A., Possega, M., Di Carlo, E., Cherchi, A., Boussetta, S., Balsamo, G., Ardilouze, C., Dayon, G., and van Oorschot, F.: Representation of Temporal Variations of Vegetation in Reanalysis and Climate Predictions: Diverging Soil-Moisture Response in Land Surface Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13385, https://doi.org/10.5194/egusphere-egu25-13385, 2025.

EGU25-14900 | ECS | Posters on site | CL4.8

Psychological Drivers of Climate Silence: A Challenge to Indonesia's Climate Action 

Anggi Dewita and Balgis Inayah

Despite growing awareness of climate change, many Indonesians remain climate-silent, posing a significant challenge to the country's efforts to mitigate its impacts. This study aims to analyze the factors contributing to climate silence in Indonesia, using psychological theories related to climate science denial. A rapid systematic review was conducted to gather evidence, revealing five key drivers of climate denial: limited cognitive abilities, ideological beliefs, sunk costs, perceived risks, and discredence. These barriers are further shaped by factors such as government policies, economic conditions, religious influences, and insufficient environmental education.
This skepticism towards climate change undermines adaptation and mitigation efforts by disrupting community engagement and participation. The findings highlight the importance of government support in addressing the root causes of climate skepticism. Employing the concept of inoculation through a misconception-based learning approach—integrated into religion and education—can help reshape mindsets. Enhancing public understanding of climate change is essential to fostering community involvement and support for effective climate mitigation initiatives.

Keywords: climate silence, climate denial, psychological drivers, Indonesia.

How to cite: Dewita, A. and Inayah, B.: Psychological Drivers of Climate Silence: A Challenge to Indonesia's Climate Action, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14900, https://doi.org/10.5194/egusphere-egu25-14900, 2025.

EGU25-15251 | Posters on site | CL4.8

Assessment of the skill of seasonal probabilistic hydrological forecasts with ParFlow/CLM over central Europe 

Alexandre Belleflamme, Suad Hammoudeh, Klaus Goergen, and Stefan Kollet

In recent years, alternating drought and extreme precipitation events have highlighted the need for subseasonal to seasonal forecasts of the terrestrial water cycle. In particular, predictions of the impacts of dry and wet extremes on subsurface water resources are crucial to provide stakeholders in agriculture, forestry, the water sector, and other fields with information supporting the sustainable use of these resources.

In this context, we release an experimental Water Resources Bulletin (https://adapter-projekt.de/bulletin/index.html) four times per year, offering probabilistic forecasts of the total subsurface water storage (TSS) anomaly at a 0.6 km resolution, from the surface down to 60 m depth, for the upcoming seven months across Germany. These seasonal forecasts are generated using the integrated, physics-based hydrological model ParFlow/CLM, forced by 50 ensemble members of the SEAS5 seasonal forecast from the European Centre for Medium-Range Weather Forecasts (ECMWF).

To evaluate our forecasts, we evaluated six 7-months probabilistic forecasts covering the vegetation period (March to September) for the years 2018 to 2023 with a reference long-term historical time series based on the same ParFlow/CLM setup. The forecast skill was assessed by comparing these seasonal forecasts to a climatology-based 10-member pseudo-forecast over the 2013–2023 period (using the leave-one-out method), extracted from the reference time series.

The monthly Continuous Ranked Probability Skill Score (CRPSS), which evaluates the ensemble distribution based on daily TSS data, indicates that the probabilistic forecast outperforms the climatology-based pseudo-forecast in most regions, except in 2018 and, to a lesser extent, in 2020 and 2022. This can be attributed to an under-representation of extremely dry members in the ensemble, combined with the memory effect of the initial conditions at increasing soil depths. For example, while March 2018 started with a slightly above-average TSS and experienced a strong meteorological drought leading to an agricultural drought, the initial TSS anomaly in March 2019 was already negative, with a less pronounced precipitation deficit during the vegetation period. This resulted in a much higher forecast skill, because of the memory effect accurately simulated with the physics-based model. Notably, the forecast skill only slightly decreases with increasing lead time, both for precipitation and TSS.

The analysis of the Relative Operating Characteristic Skill Score (ROCSS) for the lower quintile of the TSS distribution assesses whether negative TSS anomalies (i.e., droughts) are adequately represented within the probabilistic forecast ensemble. The results are consistent with those of the CRPSS, showing lower skill in 2018. Nevertheless, the ROCSS analysis overall indicates moderate to high skill for the probabilistic forecast, while the climatology-based pseudo-forecast demonstrates no skill. This confirms that the dry conditions experienced in central Europe in recent years were captured within the probabilistic forecast, underlining the added value of these forecasts and their usefulness in the experimental Water Resources Bulletin.

How to cite: Belleflamme, A., Hammoudeh, S., Goergen, K., and Kollet, S.: Assessment of the skill of seasonal probabilistic hydrological forecasts with ParFlow/CLM over central Europe, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15251, https://doi.org/10.5194/egusphere-egu25-15251, 2025.

EGU25-15484 | ECS | Posters on site | CL4.8

From Policy to Action: Empowering Women to Lead Climate Resilience in Indonesia 

Asri Rachmawati and Anggi Dewita

Women face disproportionate impacts from climate change due to significant barriers to accessing education and protection. In Indonesia, women often lack access to essential resources and opportunities, particularly in urban informal settlements. However, women also hold a pivotal position in the community in advancing climate literacy. Despite progressive regulations supporting women’s rights, gaps in implementation persist, highlighting the need for targeted initiatives to enhance women’s understanding of climate issues and their capacity to lead resilience efforts. Indonesia has established strong policies for gender equality and climate action, such as Presidential Regulation No. 59/2017 and the National Action Plan for Climate Change Adaptation (RAN-API), which emphasize gender-responsive strategies. However, translating these policies into real-world actions remains a challenge, highlighting the need to better connect scientific research and community insights to effective governance and implementation. This study identifies a critical gap in urban climate literacy and proposes empowering women as a solution. By leveraging women’s social network in Indonesia, the project disseminates climate knowledge and fosters collective action. Key initiatives include training women in climate literacy, introducing sustainable practices such as urban gardening, and developing accessible educational tools like songs, games, and visual materials. These programs are designed to position women as trusted leaders within their communities. Structured monitoring and evaluation methods, including annual surveys and peer-led literacy programs, ensure continuous improvement and scalability. Preliminary findings demonstrate that women-led climate literacy initiatives significantly enhance community resilience and resource allocation. Empowered women influence their families and peers, creating a ripple effect that strengthens societal adaptability. This scalable model integrates women-centered initiatives into governance frameworks, building pathways for sustainable, inclusive development. By empowering women, we transform vulnerability into strength, paving the way for a resilient future.

How to cite: Rachmawati, A. and Dewita, A.: From Policy to Action: Empowering Women to Lead Climate Resilience in Indonesia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15484, https://doi.org/10.5194/egusphere-egu25-15484, 2025.

EGU25-15694 | Orals | CL4.8 | Highlight

The Use of Social Media on Weather and Climate Information Dissemination To Support Effective Climate Action 

Radjab Achmad Fachri and Achmad Ezra Reynara

Timely and fast dissemination are some of the key factors for the effective climate information services in order to support effective climate action. Various mean of communication channel has been used by an authoritative agency to disseminate their climate information, including social media. Currently, social media become one of the most effective chanel to disseminate of weather and climate information. Social media is not only a powerfull tools to ensure the timely, fast, massive dissemination of weather and climate information, but it is also easy to use and access by the general public. Social media also can be optimized public outreach and public education in order to raising awareness and mobilizing an effective climate action. Through it’s real time response tools, social media also can be used to strengthen the engagement between meteorological and hydrological services with their users. Our research will describe the effectiveness of social media to disseminate weather and climate information in order to support climate action in Indonesia.

How to cite: Achmad Fachri, R. and Ezra Reynara, A.: The Use of Social Media on Weather and Climate Information Dissemination To Support Effective Climate Action, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15694, https://doi.org/10.5194/egusphere-egu25-15694, 2025.

EGU25-19049 | Posters on site | CL4.8

The Role of Afforestation in Modulating Arid Climate 

Thang M. Luong, Matteo Zampieri, and Ibrahim Hoteit

Afforestation and greening initiatives are increasingly considered viable strategies for mitigating climate change, particularly in arid regions. In this study, we assess the climate impacts of large-scale afforestation in the Arabian Peninsula (AP). The afforestation is represented by replacing sandy bare soil with woody savanna vegetation, assumed to be naturally sustained by rainfall, in the absence of overgrazing. Using a 30-year regional climate model simulation, we prescribe afforestation within a circular area of 4.5° radius (approximately 71.9 million hectares) centered at 24.2°N, 44.3°E. The afforestation modifies surface characteristics, including darker albedo (0.25 vs. 0.38 for bare soil), a green fraction of 0.3, and a leaf area index (LAI) of 0.1.

Our results show that the afforestation slows down near-surface winds and due to darker surface, increases sensible heat flux, leading to enhanced warming of the atmosphere over vegetated areas. Despite these warming effects, the additional vegetation promotes higher rainfall due to increased moisture availability and reduction of subsidence. This study underscores the dual role of afforestation in modulating regional climate, serving as both a climate mitigation measure and a potential warming source, depending on regional conditions. These findings highlight the importance of considering water availability and local climate factors when designing greening policies for arid regions.

How to cite: Luong, T. M., Zampieri, M., and Hoteit, I.: The Role of Afforestation in Modulating Arid Climate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19049, https://doi.org/10.5194/egusphere-egu25-19049, 2025.

EGU25-19889 | Orals | CL4.8

Progresses and Challenges for Subseasonal to Interdecadal Prediction 

Ángel G. Muñoz, William J. Merryfield, and Debra Hudson

Subseasonal to decadal predictions provide essential information that bridges the gap in timescales between weather forecasts and long-term climate projections. The science and practice of making such predictions using global climate models initialized with observational data has advanced considerably in recent years, and as a result operational subseasonal, seasonal and decadal prediction services are now a reality. Nonetheless, important remaining challenges must be overcome if these predictions are to more fully realize their potential value for society. This talk highlights five key challenges recommended as targets for focused international research; these are set against a backdrop of wider challenges encompassing climate modelling and services across time scales.

How to cite: Muñoz, Á. G., Merryfield, W. J., and Hudson, D.: Progresses and Challenges for Subseasonal to Interdecadal Prediction, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19889, https://doi.org/10.5194/egusphere-egu25-19889, 2025.

EGU25-21425 | Orals | CL4.8

A large ensemble of decadal predictions using MIROC6 

Takahito Kataoka, Hiroaki Tatebe, Hiroshi Koyama, and Masato: Mori

The climate fluctuates on various timescales and in various patterns, giving rise to extreme events over the globe. Skillful predictions of such climate variations would therefore benefit society, and there have been substantial efforts. For the CMIP6 Decadal Climate Prediction Project (DCPP), we performed decadal predictions with ten ensemble members using the Model for Interdisciplinary Research on Climate version 6 (MIROC6). However, since models tend to underestimate signal-to-noise ratio in some sectors, such as the Atlantic, a large ensemble size appears to be required for skillful predictions of those variations. To better understand the predictability on timescales out to a season to a decade, we have prepared a set of initialized predictions using MIROC6 that consists of 10-year-long hindcasts starting every November between 1960-2021, with 50 ensemble members. Compared to the original 10-member ensemble hindcast, both seasonal and decadal prediction skills are broadly improved (e.g., SAT and SLP over southeast China and Scandinavia for the first winter, North and South Pacific SSTs for decadal prediction). Regarding the decadal prediction skill, the impact of initialization is seen up to lead year 7-10 for the North and eastern tropical Pacific Oceans.
Also, building on our experience with decadal climate predictions, we have been working on decadal carbon predictions in recent years. Our efforts on earth system predictions will be introduced as well.

How to cite: Kataoka, T., Tatebe, H., Koyama, H., and Mori, M.: A large ensemble of decadal predictions using MIROC6, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21425, https://doi.org/10.5194/egusphere-egu25-21425, 2025.

Sea surface temperature anomalies (SSTAs) over the North Atlantic (NA) have a significant impact on the weather and climate in both local and remote regions. This study first evaluated the seasonal prediction skill of NA SSTA using the North American multi-model ensemble and found that its performance is limited across various regions and seasons. Therefore, this study constructs models based on the long short-term memory (LSTM) network machine learning method to improve the seasonal prediction of NA SSTA. Results show that the seasonal prediction skill can be significantly improved by LSTM models since they show higher capability to capture nonlinear processes such as the impact of El Nin ̃o-Southern Oscillation on NA SSTA. This study shows the great potential of the LSTM model on the seasonal prediction of NA SSTA and provides new clues to improve the seasonal predictions of SSTA in other regions.

How to cite: Yan, X. and Tang, Y.: Seasonal prediction of North Atlantic sea surface temperature anomalies using the LSTM machine learning method , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-153, https://doi.org/10.5194/egusphere-egu25-153, 2025.

EGU25-3747 | Orals | CL4.6

Bridging paleoclimate and seasonal climate prediction: The case of European summer climate 

Martin Wegmann and Stefan Brönnimann

Understanding monthly-to-annual climate variability is essential for improving climate forecast products as well as adapting to future climate extremes. Previous studies show, that European summer climate, including temperature and precipitation extremes, is modulated by hemispheric large-scale circulation patterns, which themselves are connected to Earth system components such as sea surface temperature across temporal scales. Nevertheless, it remains unclear as to how stationary these teleconnections are and if their predictive power is potent across multiple centuries and background climates. By combining d18O isotopes from a European tree ring network with independent paleo-climate reanalyses, we highlight precursors and atmospheric dynamics behind European summer climate over the last 400 years.

We further present evidence that centennial ensemble seasonal climate forecasts capture the causality of the atmospheric
dynamics behind these teleconnections in the 20th century. Our results suggest that tropical sea surface temperature anomalies trigger specific precipitation and diabatic heating patterns which are dynamically connected to extratropical Rossby wave trains and the formation of a circumglobal teleconnection pattern weeks later.

How to cite: Wegmann, M. and Brönnimann, S.: Bridging paleoclimate and seasonal climate prediction: The case of European summer climate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3747, https://doi.org/10.5194/egusphere-egu25-3747, 2025.

EGU25-3839 | ECS | Posters on site | CL4.6

Causal Links Between North Atlantic SSTs and Summer East Atlantic Pattern Predictability: Implications for Seasonal Forecasting 

Julianna Carvalho Oliveira, Giorgia Di Capua, Leonard F. Borchert, Reik V. Donner, and Johanna Baehr

We use causal effect networks to assess the influence of spring North Atlantic sea surface temperatures (NA-SSTs) on summer East Atlantic (EA) pattern predictability during 1908–2008. In the ERA-20C reanalysis, a robust causal link is identified for 1958–2008, where the spring meridional SST gradient causes a 0.2 standard deviation change in the summer EA. Additionally, the spring meridional SST index has an estimated negative causal effect (~−0.2) on summer 2m air temperatures over northwestern Europe. However, both links are absent when analysing the full period and are sensitive to interannual variability.

Analysis of the Max Planck Institute Earth System Model in mixed resolution (MPI-ESM-MR) shows that historical simulations fail to reproduce the observed causal links, while initialised ensembles occasionally capture them but underestimate their strength. Predictive skill assessments conditioned on these causal links indicate limited overall impact but suggest potential local improvements for European summer climate forecasts. These findings underscore the value of causal approaches for refining seasonal predictability.

How to cite: Carvalho Oliveira, J., Di Capua, G., Borchert, L. F., Donner, R. V., and Baehr, J.: Causal Links Between North Atlantic SSTs and Summer East Atlantic Pattern Predictability: Implications for Seasonal Forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3839, https://doi.org/10.5194/egusphere-egu25-3839, 2025.

EGU25-5880 | Orals | CL4.6

Intermittency of seasonal forecast skill for the wintertime North Atlantic Oscillation and East Atlantic Pattern  

Laura Baker, Len Shaffrey, Antje Weisheimer, and Stephanie Johnson

The wintertime North Atlantic Oscillation (NAO) and East Atlantic Pattern (EA) are the two leading modes of North Atlantic pressure variability and have a substantial impact on winter weather in Europe. The year-to-year contributions to multi-model seasonal forecast skill in the Copernicus C3S ensemble of seven prediction systems are assessed for the wintertime NAO and EA, and well-forecast and poorly-forecast years are identified. Years with high NAO predictability are associated with substantial tropical forcing, generally from the El Niño Southern Oscillation (ENSO), while poor forecasts of the NAO occur when ENSO forcing is weak. Well-forecast EA winters also generally occurred when there was substantial tropical forcing, although the relationship was less robust than for the NAO. These results support previous findings of the impacts of tropical forcing on the North Atlantic and show this is important from a multi-model seasonal forecasting perspective.

How to cite: Baker, L., Shaffrey, L., Weisheimer, A., and Johnson, S.: Intermittency of seasonal forecast skill for the wintertime North Atlantic Oscillation and East Atlantic Pattern , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5880, https://doi.org/10.5194/egusphere-egu25-5880, 2025.

EGU25-6006 | ECS | Orals | CL4.6

 Investigating the sensitivity of 20th century seasonal hindcasts to tropospheric aerosol forcing 

Matthew Wright, Antje Weisheimer, Tim Woollings, Retish Senan, and Timothy Stockdale

Previous studies have identified multi-decadal variations in the skill of winter seasonal forecasts of large-scale climate indices, including ENSO, the PNA, and NAO. Forecast skill is significantly lower in the middle of the 20th century (1940—1960) than at the start or end of the century. We hypothesise that tropospheric aerosol forcing, which is spatially and temporally heterogeneous and poorly constrained in the hindcasts used in previous studies, contributes to this low skill mid-century period.

This study assesses the sensitivity of ECMWF’s state-of-the-art seasonal forecasting model to tropospheric aerosol forcing, using a newly developed aerosol forcing dataset based on CEDS emissions data. We analyse DJF hindcasts initialised every November from 1925—2010, each with 21 ensemble members. For each year, we run hindcasts with ‘best guess’, doubled, and halved aerosol forcing (perturbing both anthropogenic and natural aerosols). All experiments exhibit similar multi-decadal variability in skill for large-scale climate indices. Aerosol forcing has no significant impact on forecast skill but some impacts on mean biases, suggesting other factors drive the mid-century skill minimum.

Aerosol forcing has large regional impacts. Increasing aerosol forcing leads to cooler 2m temperature and SSTs globally, with amplified cooling in regions with large aerosol forcings, such as northern India and North Africa. Dynamical responses include an ‘anti-monsoon’ circulation over Africa, with a weakening of the trade winds and Atlantic Walker circulation, and local southwards shift of the ITCZ. The magnitude of the response increases when ocean initial conditions are perturbed to represent the cumulative impact of aerosol forcing, suggesting that coupling enhances the atmospheric response.

These results highlight the model’s sensitivity to tropospheric aerosols, with large differences in bias and mean state after four months, despite limited impact on skill. The circulation changes over Africa warrant further investigation, with implications for future aerosol scenarios. Planned experiments will explore the impact in summer and quantify the timescale of the response to aerosols.

How to cite: Wright, M., Weisheimer, A., Woollings, T., Senan, R., and Stockdale, T.:  Investigating the sensitivity of 20th century seasonal hindcasts to tropospheric aerosol forcing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6006, https://doi.org/10.5194/egusphere-egu25-6006, 2025.

This study shows a close relationship between winter Arctic sea ice concentration (WASIC) anomalies in the Barents-Greenland Seas and the subsequent autumn Indian Ocean Dipole (IOD) based on the observational analysis and numerical simulations. Particularly, more (less) WASIC in the Barents-Greenland Seas tends to lead to a positive (negative) IOD in the following autumn. Above-normal WASIC in the Barents-Greenland Seas results in reduction of the upward turbulent heat flux and induces tropospheric cooling over the Arctic. This tropospheric cooling triggers an atmospheric teleconnection extending from the Eurasian Arctic to the subtropical North Pacific. Numerical experiments with both the linear barotropic model and atmospheric general circulation model can well capture the atmospheric teleconnection associated with the WASIC anomalies. The subtropical atmospheric anomalies generated by the WASIC anomalies then result in subtropical sea surface temperature (SST) warming, which sustains and expands southward to the equatorial central Pacific during the following summer via a wind-evaporation-SST feedback. The resulting equatorial central Pacific SST warming anomalies induce local atmospheric heating and trigger an anomalous Walker circulation with descending motion and low-level anomalous southeasterly winds over the southeastern tropical Indian Ocean. These anomalous southeasterly winds trigger positive air-sea interaction in the tropical Indian Ocean and contribute to the development of the IOD. The close connection of the WASIC anomalies with the subsequent IOD and the underlying physical processes can be reproduced by the coupled climate models participated in the CMIP6. These results indicate that the condition of WASIC is a potential effective precursor of IOD events.

How to cite: Xin, C.: Influence of winter Arctic sea ice anomalies on the following autumn Indian Ocean Dipole development, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6176, https://doi.org/10.5194/egusphere-egu25-6176, 2025.

EGU25-7163 | Orals | CL4.6

Robust decadal predictability of cold surge frequency in Taiwan and East Asia through teleconnection of North Atlantic Oscillation 

Wan-Ling Tseng, Yi-Chi Wang, Ying-Ting Chen, Yi-Hui Wang, Huang-Hsiung Hsu, and Chi-Cherng Hong

This study investigates the decadal predictability of cold surge frequency (CSF) in East Asia, including Korea, Japan, and Taiwan, through the lens of the North Atlantic Oscillation (NAO) index. The findings suggest that extreme events such as cold surges can be predicted on decadal timescales when the teleconnection mechanism is robustly established. The study revisits and consolidates the dynamical mechanisms underlying wave propagation and the teleconnection between the NAO and the East Asian trough, highlighting their role in creating a winter environment conducive to cold surges in Taiwan and East Asia. The study demonstrates the skill of climate models in capturing the NAO's decadal variability, and develops a statistical-dynamical hybrid approach. This method integrates decadal prediction datasets with a statistical model to enhance the prediction of extreme cold surge occurrences on a multi-annual timescale. The results of the study underscore the scientific significance of merging climate dynamical mechanisms with decadal prediction systems for extreme events, and introduce a hybrid framework that combines numerical decadal climate predictions with statistical regression models. This addresses the challenges posed by biases in climate prediction models and advances the capability to predict regional extreme events such as cold surges.

How to cite: Tseng, W.-L., Wang, Y.-C., Chen, Y.-T., Wang, Y.-H., Hsu, H.-H., and Hong, C.-C.: Robust decadal predictability of cold surge frequency in Taiwan and East Asia through teleconnection of North Atlantic Oscillation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7163, https://doi.org/10.5194/egusphere-egu25-7163, 2025.

EGU25-8693 | ECS | Orals | CL4.6

Decadal prediction for the European Energy Sector 

Benjamin Hutchins, David Brayshaw, Len Shaffrey, Hazel Thornton, and Doug Smith

The timescale of decadal climate predictions, from a year-ahead up to a decade, is an important planning horizon for stakeholders in the energy sector. With power systems transitioning towards a greater share of renewables, these systems become more vulnerable to the impacts of both climate variability and climate change. As decadal predictions sample both the internal variability of the climate and the externally forced response, these forecasts can provide useful information for the upcoming decade. 

There are two main ways in which decadal predictions can benefit the energy sector. Firstly, they can be used to try to predict how a variable of interest, such as average temperature, may evolve over the coming year or decade. Secondly, a large ensemble of decadal predictions can be aggregated into a large synthetic event set to explore physically plausible extremes, such as winter wind droughts. 

We find predictive skill at decadal timescales for surface variables over Europe during both winter (ONDJFM) and summer (AMJJAS). Although this skill is patchy, there are regions of relevance to the energy sector, such as over the UK for temperature, where this skill emerges. We find significant skill when using pattern-based (e.g., NAO) approaches to make predictions of European energy indicators during the extended winter, including Northern Europe offshore wind generation, Spanish solar generation, and Scandinavian precipitation. For predicting UK electricity demand, we find significant skill when directly using the model predictions of surface temperature. Our results highlight the potential for operational decadal predictions for the energy system, with potential benefits for both the planning and operation of the future power system. 

How to cite: Hutchins, B., Brayshaw, D., Shaffrey, L., Thornton, H., and Smith, D.: Decadal prediction for the European Energy Sector, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8693, https://doi.org/10.5194/egusphere-egu25-8693, 2025.

EGU25-8904 | Orals | CL4.6

On the predictive skill for warm spells in Germany across seasons  

Fabiana Castino, Tobias Geiger, Alexander Pasternack, Andreas Paxian, Clementine Dalelane, and Frank Kreienkamp

Intense warm spells, such as heatwaves, can significantly impact human health, the environment, and socio-economic systems. Although heatwaves are typically associated with summer, the occurrence of warm spells during cold seasons can also have profound effects on various sectors. While some effects, such as reduced cold-related mortality, can be considered beneficial, the long-term consequences, e.g. on ecosystems, forests, and agriculture, are concerning. Warm spells during the cold seasons can alter the natural dormancy cycles of plants, causing premature sprouting, flowering, or growth and negatively affecting crop yield and quality. In addition, cold season warm spells can reduce snow accumulation in mountainous regions, potentially affecting downstream water availability. As climate change drives increases in the frequency, intensity, and duration of warm spells, their impacts are becoming more severe and far-reaching. This makes predicting such events a key priority for climate science and risk management.

Climate forecast models offer the potential to predict extreme events like warm spells weeks to months in advance, becoming increasingly relevant for decision-making across various socio-economic sectors. This study examines the predictive skill of the downscaled German Climate Forecast System Version 2.1 (GCFS2.1) for warm spells in Germany on a seasonal scale, encompassing both warm seasons (spring and summer) and cold seasons (autumn and winter).  The analysis relies on hindcast data from the 1991-2020 base period, statistically downscaled to 5 km resolution. It evaluates multiple extreme temperature climate indices, as for example the Warm Spells Duration index, and applies various statistical metrics to assess the predictive skill. The findings reveal high heterogeneity in the ability of the (downscaled) GCFS2.1 to forecast warm spells across seasons, with higher predictive skill during the cold seasons but more limited for the warm seasons.

How to cite: Castino, F., Geiger, T., Pasternack, A., Paxian, A., Dalelane, C., and Kreienkamp, F.: On the predictive skill for warm spells in Germany across seasons , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8904, https://doi.org/10.5194/egusphere-egu25-8904, 2025.

EGU25-8980 | ECS | Orals | CL4.6

Predicting North Atlantic Temperature Trends with the Analogue Method using the MPI CMIP6 Grand Ensemble 

Lara Heyl, Sebastian Brune, and Johanna Baehr

The analogue method is a powerful and efficient tool for climate predictions, particularly in regions like the North Atlantic, where impacts of climate change have been relatively modest. While climate projections effectively estimate global mean surface temperature trends over a century, decadal trends in the North Atlantic diverge from the global trend. Here, we leverage on the similar evolution of analogous patterns on a decadal time scale by comparing SST patterns in observed data with patterns from an existing simulation ensemble. We apply this method to ten-year SST trend reconstructions in the North Atlantic using the MPI CMIP6 grand ensemble. In addition, we assess the impact of volcanic eruptions on the quality of the SST trend reconstruction for the time period 1960-2019. We also provide a prediction for 2020–2029. We find that the analogue method delivers high correlation of SST trend reconstructions with observed trends for the MPI CMIP6 grand ensemble. Volcanic influence can be accounted for by trimming the time series to those times unaffected by volcanic eruptions, which results in a higher correlation. Our results suggest that the decadal predictions of SST trends might also be achieved without the need for new, computationally expensive simulations.

How to cite: Heyl, L., Brune, S., and Baehr, J.: Predicting North Atlantic Temperature Trends with the Analogue Method using the MPI CMIP6 Grand Ensemble, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8980, https://doi.org/10.5194/egusphere-egu25-8980, 2025.

EGU25-9006 | Posters on site | CL4.6

Is the winter mean NAO white noise? Models and observations. 

Bo Christiansen and Shuting Yang

The NAO is a dominant mode of variability in the Northern Hemisphere with strong impacts on temperature, precipitation, and storminess. The predictive skill of the NAO on annual to decadal scales is therefore an important topic, which is often studied using, e.g., (initialized) climate models. The temporal structure is closely related to the predictability, and on inter-annual time scales the observed NAO is frequently described to have power at 2-7 years and sometimes with a distinct peak around 7 or 8 years.  However, the observational record is brief, and such estimations have high uncertainty.

Here, we present a thorough study to answer the questions: is the winter mean NAO different from white noise and is the observed NAO different from the NAO in historical experiments with contemporary climate models (CMIP6)? To this end we use a range of statistical tools in both the temporal and spectral domain: Power-spectra, wavelet-spectra, autoregressive models, and various well-known time-series statistics.

Overall, we find little evidence to reject that the NAO is white noise. For observations, the peak in the power-spectrum at 8 years is, taken individually, significant in the period after 1950 but not before. However, considering the complete spectrum, significant peaks will often occur at some frequency, even for white noise.  The large CMIP6 multi-model ensemble is statistically very similar to an ensemble of similar size of white noise, e.g., the ensemble averages of the power spectrum and the wavelet spectra are completely flat.  Furthermore, for both observations and the model ensemble the tests based on autoregressive modelling and time-series statistics do not reject the null-hypothesis of white noise.

How to cite: Christiansen, B. and Yang, S.: Is the winter mean NAO white noise? Models and observations., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9006, https://doi.org/10.5194/egusphere-egu25-9006, 2025.

EGU25-10305 | ECS | Posters on site | CL4.6

Towards improved forecast initialisations with an observation-informed ocean grid 

Marlene Klockmann, Kai Logemann, Sebastian Brune, and Johanna Baehr

For climate forecasts it is crucial to initialise the ocean state from observations because they rely on the memory of the ocean. If, however, the initialised ocean state is far away from the model’s own preferred mean state, predictive skill will suffer due to model drift. We are testing whether an ocean grid with variable resolution - designed to represent sparse and well-observed regions with appropriate resolution - has advantages over an ordinary grid with uniform resolution. The locally high resolution could lead to an improved mean ocean state through a better representation of mesoscale processes. The observation-informed grid will allow for high-resolution data assimilation in well-observed areas, which will potentially lead to improved initial conditions and predictive skill.  

We developed such a grid for the ocean component of the coupled ICON model designed for seamless predictions (ICON-XPP). The grid resolution varies from 40 to 10km, depending on the observation density in the EN4 database from 1960 to 2023. The local refinement in well-observed areas leads to a better representation of ocean features such as fronts and western boundary currents. We assess the effect of these improvements on the mean climate state by comparing to a reference simulation with a uniform 20km ocean resolution. 

 

How to cite: Klockmann, M., Logemann, K., Brune, S., and Baehr, J.: Towards improved forecast initialisations with an observation-informed ocean grid, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10305, https://doi.org/10.5194/egusphere-egu25-10305, 2025.

EGU25-10747 | Posters on site | CL4.6

Ocean–atmosphere feedbacks key to NAO decadal predictability 

Panos J. Athanasiadis, Casey Patrizio, Doug M. Smith, and Dario Nicolì

Recent studies using initialised large-ensemble re-forecasts have shown that the North Atlantic Oscillation (NAO) exhibits significant decadal predictability, which is of great importance to society given the significant climate anomalies that accompany the NAO. However, the key physical processes underlying this predictability, including the role of ocean–atmosphere interactions, have not yet been pinned down. Also, a critical deficiency in the representation of the associated predictable signal by climate models has been identified in recent studies (the signal-to-noise problem), still lacking an explanation.

In this study, the decadal prediction skill for the NAO and the interactions of the associated atmospheric circulation anomalies with the underlying ocean are assessed using retrospective forecasts from eight decadal prediction systems and observation-based data. We find considerable spread in the NAO skill across these systems and critically, that this is linked to differences in the representation of ocean–NAO interactions across the systems. Evidence is presented that the NAO skill depends on a direct positive feedback between subpolar sea surface temperature anomalies and the NAO, which varies in strength across the prediction systems, yet may still be too weak even in the most skillful systems compared to the observational estimate. This positive feedback is opposed by a delayed negative feedback between the NAO and the ocean circulation that also contributes to disparities in the NAO skill across systems. Our findings therefore suggest that North Atlantic ocean–atmosphere interactions are central to NAO decadal predictability. Finally, it is suggested that errors in the representation of these interactions may be contributing significantly to the signal-to-noise problem.

How to cite: Athanasiadis, P. J., Patrizio, C., Smith, D. M., and Nicolì, D.: Ocean–atmosphere feedbacks key to NAO decadal predictability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10747, https://doi.org/10.5194/egusphere-egu25-10747, 2025.

EGU25-10815 | Posters on site | CL4.6

Planktonic foraminifera as a tool of past seasonality reconstruction 

Zhoufei Yu, Baohua Li, and Shuai Zhang

Seasonal changes in seawater temperature leave large imprints on the stable oxygen isotope composition (δ18O) of planktonic foraminiferal tests, based on which the past seasonal changes can be reconstructed. However, there are still problems needed to be figured out in regard to this new method, to improve the reliability of seasonality reconstruction. For example, the selected foraminiferal species, the used size fraction, and the sample area. As a result, by analyzing planktonic foraminiferal test δ18O from the sediment trap samples deployed in the South China Sea, we found that foraminiferal seasonal δ18O signal is strongly distorted (amplified or damped) by seasonal variations in their habitat depth, particularly for the species living in low latitude. Furthermore, Globigerinoides ruber of 300-355 um can record the most comprehensive seawater seasonality information. This study provides strong support to the reconstruction of past seawater seasonal temperature by using individual planktonic foraminifera.

How to cite: Yu, Z., Li, B., and Zhang, S.: Planktonic foraminifera as a tool of past seasonality reconstruction, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10815, https://doi.org/10.5194/egusphere-egu25-10815, 2025.

EGU25-11024 | ECS | Orals | CL4.6

Skill assessment of a multi-system ensemble of initialized 20-year predictions 

Dario Nicolì, Sebastiano Roncoroni, Wolfgang A. Mueller, Holger Pohlmann, Sebastian Brune, Markus Donat, Rashed Mahmood, Steve Yeager, William J. Merryfield, Reinel Sospedra-Alfonso, and Panos J. Athanasiadis

Decadal predictions have advanced greatly in recent years: not only have they become operational worldwide and have been demonstrated to be skillful in various aspects of climate variability, including predicting changes in the atmospheric circulation and in the occurrence of extremes several years ahead, but —as such— they are also being used increasingly in climate services. Climate adaptation and policy making, however, also require climate predictions that go beyond the 10-year horizon. For climate information beyond 10 years into the future, uninitialized climate projections, which completely miss any predictability stemming from internal variability, have been the only available product. Trying to account for this lack of information in climate projections regarding any predictable components of internal variability, methods to constrain climate projections using information from large ensembles of initialized decadal predictions have been developed and have been shown to reduce the uncertainty and increase the skill of climate projections, even beyond the 10-year horizon. The demonstrated benefits of such indirect methods to account for predictable internal variability indicate that the latter remains significant beyond the 10-year limit of decadal predictions. Hence, directly harnessing this predictability through running initialized 20-year predictions emerges as a strategic endeavour.
In this study a novel, multi-system ensemble of initialized extended-decadal predictions is assessed. These predictions consist of a grand ensemble of 71 members derived from 6 forecast systems. They are initialized every 5 years from 1960 onward and run ahead for 20 years. Our analysis uses an elaborate drift- and bias-correction method that accounts for the correct representation of trends. Importantly, we show significant skill against observations for a number of variables (fields and indices), even in the second decade of the forecasts. The origin of such predictability is discussed together with the limitations of these 20-year predictions. The respective experimental protocol was defined in the framework of the ASPECT EU project and has been proposed as a tier-2 Decadal Climate Prediction Project (DCPP) protocol for the Coupled Model Intercomparison Project phase 7 (CMIP7).

How to cite: Nicolì, D., Roncoroni, S., Mueller, W. A., Pohlmann, H., Brune, S., Donat, M., Mahmood, R., Yeager, S., Merryfield, W. J., Sospedra-Alfonso, R., and Athanasiadis, P. J.: Skill assessment of a multi-system ensemble of initialized 20-year predictions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11024, https://doi.org/10.5194/egusphere-egu25-11024, 2025.

EGU25-11166 | ECS | Orals | CL4.6

Multidecadal variability of the ENSO teleconnection to Europe in early-winter and implications for seasonal forecasting 

Pablo Fernández-Castillo, Teresa Losada, Belén Rodríguez-Fonseca, Diego García-Maroto, Elsa Mohino, and Luis Durán

El Niño-Southern Oscillation (ENSO) is the leading mode of global climate variability. Through its associated teleconnections, ENSO can impact the climate of numerous regions worldwide at seasonal timescales, highlighting its role as the main source of seasonal predictability. Numerous studies have demonstrated a significant influence of ENSO on the climate of the Euro-Atlantic sector, but the impacts and mechanisms of the teleconnection in early-winter (November-December) remain unclear. Besides, in early-winter, ENSO teleconnections involve tropospheric pathways, which may change in response to different background states of the ocean. Thus, a crucial research question to address is whether the early-winter teleconnection to the Euro-Atlantic sector has changed under the different background states of sea surface temperature (SST) over the Pacific Ocean. 

 

This work aims to analyse the ENSO early-winter teleconnection to the Euro-Atlantic sector from a nonstationary perspective. Specifically, the teleconnection is analysed under different background states of SST over the Pacific Ocean, related to changes in the phase of the Pacific Decadal Oscillation (PDO). Using observational and reanalysis datasets for the period 1950-2022, results reveal that the tropospheric pathways of the teleconnection change under the different Pacific SST background states, leading to distinct responses of the North Atlantic atmospheric circulation to ENSO. We also confirm that these distinct responses in the North Atlantic entail significantly different impacts of ENSO on the surface climate across Europe, particularly on surface air temperature. Furthermore, the teleconnection is analysed in the SEAS5 state-of-the-art dynamical seasonal prediction model. The analysis within the model is also conducted from a nonstationary perspective, and aims to determine whether the model successfully reproduces a shift in the teleconnection in the late 1990s identified in reanalysis and observations. Results show that the model accurately captures the spatial pattern of the teleconnection impacts across Europe after the late 1990s, but not before. In turn, significant changes in the skill of seasonal forecasts are observed between before and after the late 1990s. However, skill after the late 1990s is just moderate due to a significant underestimation of the teleconnection impacts. 

 

The results of this study shed light on the nonstationary behaviour of the early-winter teleconnection to the Euro-Atlantic sector and have important implications on seasonal predictability in Europe. Particularly, the nonstationarity of the teleconnection gives rise to the emergence of windows of opportunity for seasonal forecasting, in which forecast skill may be greater than initially expected from a stationary analysis.

How to cite: Fernández-Castillo, P., Losada, T., Rodríguez-Fonseca, B., García-Maroto, D., Mohino, E., and Durán, L.: Multidecadal variability of the ENSO teleconnection to Europe in early-winter and implications for seasonal forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11166, https://doi.org/10.5194/egusphere-egu25-11166, 2025.

EGU25-11511 | Orals | CL4.6

Constraining near-term climate projections by combining observations with decadal predictions 

Rémy Bonnet, Julien Boé, and Emilia Sanchez

Reducing the uncertainty associated with internal climate variability over the coming decades is crucial, as this time frame aligns with the strategic planning needs of stakeholders in climate-vulnerable sectors. Three sources of information are available: non-initialized ensembles of climate projections, initialized decadal predictions, and observations. Non-initialized ensembles of climate projections span seamlessly from the historical period to the end of the 21st century, encompassing the full range of uncertainty linked to internal climate variability. Initialized decadal predictions aim to reduce uncertainty from internal climate variability by initializing model simulations with observed oceanic states, phasing the simulated and observed climate variability modes. However, they are usually limited to 5 to 10 years, with small added value after a few years, and they are also subject to drift due to the shock from the initialization. Finally, we can also use observations that can provide information to constrain the climate evolution over the next decades. Providing the best climate information at regional scale over the next decades is therefore challenging. Previous methods addressed this challenge by using information from either the observations or the decadal predictions to constrain uninitialized projections. In this study, we propose a new method to make use of the different sources of information available to provide relevant information about near-term climate change with reduced uncertainty related to internal climate variability. First, we select a sub-ensemble of non-initialized climate simulations based on their similarity to observed predictors with multi-decadal signal potential over Europe, such as Atlantic multi-decadal variability (AMV). Then, we further refine this sub-ensemble of trajectories by selecting a subset based on its consistency with decadal predictions. We present a case study focused on predicting near-term future surface temperatures over Europe. To evaluate the effectiveness of this method in providing reliable climate information, we conduct a retrospective analysis over the historical period.

How to cite: Bonnet, R., Boé, J., and Sanchez, E.: Constraining near-term climate projections by combining observations with decadal predictions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11511, https://doi.org/10.5194/egusphere-egu25-11511, 2025.

EGU25-12107 | Orals | CL4.6

Overcoming the spring predictability barrier with a supermodel 

Noel Keenlyside, Tarkeshwar Singh, Ping-Gin Chiu, Francois Counillon, and Francine Schevenhoven

Climate models suffer from long-standing biases that degrade climate prediction skills. While radically increasing resolution offers promise, we are still many years away from being able to perform operational climate predictions with models that can explicitly resolve the most important physical processes. Here we demonstrate that supermodelling can enhance climate predictions through better using the current generation of models. A supermodel connects different models interactively so that their systematic errors compensate. It differs from the standard non-interactive multi-model ensembles, which combines model outputs a-posteriori. We have developed an ocean-connected Earth System model using NorESM, CESM, and MPIESM in their CMIP5 versions. The model radically improves the simulation of tropical climate, strongly reducing SST and double ITCZ biases. We perform seasonal predictions for the period 1990-2020, initialized through (EnOI) data assimilation of SST. We have performed one forecast per season but are currently extending the ensemble size to ten members. The supermodel shows marked improvement in prediction skill for forecasts started before boreal spring, significantly overcoming the spring predictability barrier. Initial investigation indicates the skill enhancement is connected to better simulation of ocean-atmosphere interaction during the first part of the year, which also leads to improved initial conditions. Our results indicate the importance of better representing the signal-to-noise in the western and central Pacific during boreal spring.

How to cite: Keenlyside, N., Singh, T., Chiu, P.-G., Counillon, F., and Schevenhoven, F.: Overcoming the spring predictability barrier with a supermodel, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12107, https://doi.org/10.5194/egusphere-egu25-12107, 2025.

EGU25-12143 | Posters on site | CL4.6

Probabilistic climate outcomes from prediction aggregation 

Robin Lamboll, Sofia Palazzo Corner, and Moritz Schwarz

Currently, much of the literature around the Paris Agreement, Paris Compliance and manging the transition to net zero requires heavy use of integrated assessment models (IAMs). IAMs provide economic projections of future emissions, conditional on idealised scenarios. However, for most adaptation and cost-benefit analysis, policymakers require predictions, which IAMs do not even attempt to provide. How can we use aggregated estimates of emissions and resulting climate change to give probability distributions of climate impacts? We outline why human computation likely out-performs other prediction methods and present a flexible method to collect intended predictions from a variety of people to effectively estimate future emissions, temperatures and climate impacts via prediction aggregation platforms. These can subsequently be used to inform estimates of climate impacts. It can also highlight deficiencies in the IAM scenarios literature and indicate relative probabilities of scenarios. We estimate all-uncertainty temperatures in 2050 and outline extensions of the work.

How to cite: Lamboll, R., Palazzo Corner, S., and Schwarz, M.: Probabilistic climate outcomes from prediction aggregation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12143, https://doi.org/10.5194/egusphere-egu25-12143, 2025.

EGU25-12247 | ECS | Orals | CL4.6

Forecasting monthly-to-seasonal sea surface temperatures and marine heatwaves with graph neural networks and diffusion methods 

Varvara Vetrova, Ding Ning, Karin Bryan, and Yun Sing Koh

Knowing future sea surface temperature (SST) patterns play a crucial role not only in industries such as fisheries, shipping and tourism but also in conservation of marine species . For example, DNA of endangered species can be sampled prior to anticipated marine heatwaves to preserve marine biodiversity. Overall, availability of SST forecasts allows to mitigate potential adverse impacts of extreme events such as marine heatwaves. 

There is a strong interest in accurate forecasts of SST and their anomalies on various time scales. The commonly used approaches include physics-based models and machine learning (ML) methods. The first approach is computationally intensive and limited to shorter time scales. While several attempts have been made by the community to adapt ML models to SST forecasts several challenges still remain. These challenges include improving accuracy for longer lead SST anomaly forecasts. 

Here we present an integrated deep-learning based approach to the problem of SST anomalies and MHW forecasting. On one hand, we capitalise both on inherent climate data structure and recent advances in the field of geometric deep learning. We base our approach on a flexible architecture of graph neural networks, well suited for representing teleconnections. From another hand, we adapt the diffusion method to increase lead time of the forecasts.  Our integrated approach allows marine heatwave forecasts up to six months in advance.

How to cite: Vetrova, V., Ning, D., Bryan, K., and Koh, Y. S.: Forecasting monthly-to-seasonal sea surface temperatures and marine heatwaves with graph neural networks and diffusion methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12247, https://doi.org/10.5194/egusphere-egu25-12247, 2025.

The expansion of and increasing dependency on renewable energy that exploit climate variables, such as wind and precipitation, are highly sensitive to climate variability and weather extremes. Climate Futures is a Center of Research-based Innovation that aims to “co-produce new and innovative solutions for predicting and managing climate risks from sub-seasonal-to-seasonal (S2S) and seasonal-to-decadal (S2D) time scales with a cluster of partners in climate- and weather-sensitive sectors, including the renewable energy sector, through long-term cooperation between businesses, public organizations and research groups.

The aim of the cross-sectoral collaboration is for renewable energy companies to integrate improved climate predictions into their decision making. The long-term implications are a more resilient energy sector and stable power production. Examples of ongoing projects within the center include (1) using large ensemble climate model simulations to estimate near-future changes in precipitation variability, and (2) estimating future wind power production and variability using state-of-the-art decadal climate predictions. These results are important for future wind- and hydropower operations and infrastructure planning.

How to cite: Svendsen, L.: Climate services for and with the renewable energy sector in Norway, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12574, https://doi.org/10.5194/egusphere-egu25-12574, 2025.

EGU25-13076 | Posters on site | CL4.6

Usage of seasonal forecasts in Tropical Cyclone risk models 

Rudy Mustafa, Ulysse Naepels, Hugo Rakotoarimanga, Rémi Meynadier, and Clément Houdard

Tropical cyclones (TCs) pose significant risks to lives, infrastructure and economies, especially in coastal areas.

AXA has been developing stochastic natural hazard models (also called natural catastrophe or NatCat models) to quantify the impact of events such as TCs on its portfolios. However, NatCat models tend to model the average annual risk for a given peril. NatCat models do not consider the present state of the atmosphere and therefore are not conditioned with respect to the current tropical cyclone season.

Information about the TC risk in the upcoming weeks or months of a season could be crucial for an insurer, especially regarding its reinsurance coverage, but also for better risk mitigation through reinforced and more efficient prevention systems.

Previous studies have demonstrated that ensemble seasonal forecasts have skill in predicting TC occurrence several weeks in advance. We explore the ability of ensemble seasonal forecasts to provided skilled information on the general activity of the season to come for various lead-times (number of occurrences, number of landfalls, ACE…) and how can NatCat models be adapted to provide a more dynamic vision of the TC risk.

How to cite: Mustafa, R., Naepels, U., Rakotoarimanga, H., Meynadier, R., and Houdard, C.: Usage of seasonal forecasts in Tropical Cyclone risk models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13076, https://doi.org/10.5194/egusphere-egu25-13076, 2025.

EGU25-13668 | Orals | CL4.6

Forecasting the annual CO2 rise at Mauna Loa 

Richard Betts, Chris Jones, Jeff Knight, John Kennedy, Ralph Keeling, Yuming Jin, James Pope, and Caroline Sandford

For the last 9 years, the Met Office has issued forecasts of the annual increment in atmospheric carbon dioxide measured at Mauna Loa, accounting for both anthropogenic emissions and the effects of El Niño Southern Oscillation (ENSO) on natural carbon sinks and sources. The first forecast was produced when the 2015-2016 El Niño was emerging, and correctly predicted the largest annual CO2 increment on record at the time. In most years, the inclusion of ENSO provides a more skilful forecast than just considering emissions alone, except for 2022-2023 when La Niña conditions in late 2022 were followed by an early emergence of El Niño conditions in the second quarter of 2023. The impacts of interannual differences in emissions on the CO2 rise are usually smaller than those of ENSO variability, except in 2020 when the emergence of an unexpected large drop in global emissions due to societal responses to the COVID-19 pandemic required the forecast to be re-issued with a new estimate of the annual profile of emissions. Our forecast methodology also provides a simple means of tracking the changes in anthropogenic contributions to the annual atmospheric CO2 rise against policy-relevant scenarios. The Met Office forecast for 2023-2024 predicted a relatively large annual CO2 rise, but the observed rise was even larger, with exceptional wildfires in the Americas a likely contributor to the additional increase. Even without the effects of El Niño and other climatic influences on carbon sinks, the human-driven rise in CO2 in 2023-2024 would have been too fast to remain compatible with IPCC AR6 scenarios that limit global warming to 1.5°C with little or no overshoot. While the 2024-2025 rise is predicted to be smaller than 2023-2024, it will still be above these 1.5°C scenarios.

How to cite: Betts, R., Jones, C., Knight, J., Kennedy, J., Keeling, R., Jin, Y., Pope, J., and Sandford, C.: Forecasting the annual CO2 rise at Mauna Loa, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13668, https://doi.org/10.5194/egusphere-egu25-13668, 2025.

EGU25-13771 | Posters on site | CL4.6

Seasonal forecasting of East African short rains 

Giovanni Liguori, Agumase Kindie Tefera, William Cabos, and Antonio Navarra

The variability of East African Short Rains (October-December) has profound socioeconomic and environmental impacts on the region, making accurate seasonal rainfall predictions essential. We evaluated the predictability of East African short rains using model ensembles from the multi-system seasonal retrospective forecasts from the Copernicus Climate Change Service (C3S). We assess the prediction skill for 1- to 5-month lead times using forecasts initialized in September for each year from 1993 to 2016. Although most models exhibit significant mean rainfall biases, they generally show skill in predicting OND (October-December) precipitation anomalies across much of East Africa. However, skill is low or absent in some northern and western parts of the focus area. Along the East African coasts near Somalia and over parts of the western Indian Ocean, models demonstrate skill throughout the late winter (up to December-February), likely due to the persistence of sea surface temperature anomalies in the western Indian Ocean. Years when models consistently outperform persistence forecasts typically align with the mature phases of El Niño Southern Oscillation (ENSO) and/or Indian Ocean Dipole (IOD). This latter mode, when tracked using the Dipole Mode Index, is generally able to predict the sign of the rainfall anomaly in all models. Despite East Africa's proximity to the west pole of the IOD, the correlation between short rains and IOD maximizes when both east and west are considered. This finding confirms previous studies based on observational datasets, which indicate that broader-scale IOD variability associated with changes in the Walker Circulation, rather than local SST fluctuations, is the primary driver behind East African rainfall.     

How to cite: Liguori, G., Tefera, A. K., Cabos, W., and Navarra, A.: Seasonal forecasting of East African short rains, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13771, https://doi.org/10.5194/egusphere-egu25-13771, 2025.

EGU25-13847 | ECS | Posters on site | CL4.6

Decadal Predictions with Diffusion Models: Combining Machine Learning and Earth System Modelling 

Simon Lentz, Johanna Baehr, Christopher Kadow, Johannes Meuer, Felix Oertel, and Bijan Fallah

In the past years, decadal prediction systems have started to fill the gap between seasonal forecasts and long-term climate projections. Despite huge progress in predictive skill and decadal predictions outperforming climate projections in almost all forecast tasks, decadal predictions still possess large rooms for improvement. Machine learning based forecast systems have already outperformed traditional weather forecast systems in recent years. Similarly, machine learning has successfully transformed or assisted in data assimilation or climate data reconstruction tasks. Despite its success in the climate sciences, machine learning methods have not yet been successfully integrated in decadal prediction systems.

Combining machine learning and numerical modeling, we attempt to produce decadal climate predictions utilizing Diffusion Models, essentially probabilistic neural networks. We use such a neural network to predict global 2m-air temperatures by training it on the historical MPI-ESM-LR Grand Ensemble and finetuning it on the MPI-ESM-LR decadal predictions and on ERA5 reanalyses. The resulting predictions are qualitatively comparable to the standard MPI-ESM-LR decadal prediction system, surpassing their predictive skill for leadyears 1 and 2. With diffusion models still new to climate predictions, we expect this result to stand only at the beginning of further machine learning integration into climate predictions in general and decadal predictions in particular.

How to cite: Lentz, S., Baehr, J., Kadow, C., Meuer, J., Oertel, F., and Fallah, B.: Decadal Predictions with Diffusion Models: Combining Machine Learning and Earth System Modelling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13847, https://doi.org/10.5194/egusphere-egu25-13847, 2025.

EGU25-15772 | Orals | CL4.6

A perfect-model perspective on the signal-to-noise paradox in initialized decadal climate predictions 

Markus G. Donat, Rashed Mahmood, Francisco J. Doblas-Reyes, and Etienne Tourigny

Initialized climate predictions are skillful in predicting regional climate conditions in several parts of the globe, but also suffer from different issues arising from imperfect initializations and inconsistencies between the model and the real world climate and processes. In particular, a so-called signal-to-noise paradox has been identified in recent years. This ‘paradox’ implies that the models can predict observations with higher skill than they predict themselves, despite some physical inconsistencies between modeled and real world climate. This is often interpreted as an indicator of model deficiencies.

Here we present a perfect-model decadal prediction experiment, where the predictions have been initialized using climate states from the model's own transient simulation. This experiment therefore avoids issues related to model inconsistencies, initialization shock and the climate drift that affect real-world initialized climate predictions. We find that the perfect-model decadal predictions are highly skillful in predicting the near-surface air temperature and sea level pressure of the reference run on decadal timescales. Interestingly, we also find signal-to-noise issues, meaning that the perfect-model reference run is predicted with higher skill than any of the initialized prediction members with the same model. This suggests that the signal-to-noise paradox may not be due just to model deficiencies in representing the observed climate in initialized predictions, but other issues that affect the statistical properties of the predictions. We illustrate that this signal-to-noise problem is related to analysis practices that concatenate time series from different discontinuous initialized simulations, which introduces inconsistencies compared to the continuous transient climate realizations and the observations. In particular, the concatenation of predictions initialized independently into a single time series breaks the auto-correlation of the time series.

How to cite: Donat, M. G., Mahmood, R., Doblas-Reyes, F. J., and Tourigny, E.: A perfect-model perspective on the signal-to-noise paradox in initialized decadal climate predictions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15772, https://doi.org/10.5194/egusphere-egu25-15772, 2025.

EGU25-18643 | Orals | CL4.6

Extending the Lead Time for European Winterstorm Activity Predictions 

Gregor C. Leckebusch, Kelvin S. Ng, Ryan Sriver, Lisa Degenhardt, Eleanor Barrie, and Elisa Spreitzer

The most dangerous and costly meteorological hazards in Europe are extreme extra-tropical cyclones and associated windstorms (EUWS) in winter. Recent studies have shown that seasonal prediction systems can skilfully predict the seasonal frequency of EUWS with a one-month lead time using November initialisations. Given that many seasonal prediction systems produce seasonal forecasts at the start of each month, this raises the question whether pre-November initialised seasonal forecasts could provide usable information in predicting seasonal activity of EUWS.

In this study, we will present preliminary results of an approach aimed at extending the predictive horizon of seasonal EUWS activity. While the direct outputs of the pre-November initialised seasonal predictions of EUWS do not have the sufficient skill, skilful predictions of seasonal EUWS activity can be obtained by an approach that utilises the information of the upper ocean mean potential temperature from seasonal prediction systems. Based on our approach, skilful predictions of seasonal EUWS activity becomes possible as early as October.

How to cite: Leckebusch, G. C., Ng, K. S., Sriver, R., Degenhardt, L., Barrie, E., and Spreitzer, E.: Extending the Lead Time for European Winterstorm Activity Predictions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18643, https://doi.org/10.5194/egusphere-egu25-18643, 2025.

Long-range winter predictions over the Euro-Atlantic sector have demonstrated significant skill but suffer from systematic signal-to-noise errors. Here, we examine sources of early winter seasonal predictability in across state-of-the-art seasonal forecasting systems. As in previous studies, these systems demonstrate skill in the hindcasts of the large-scale atmospheric circulation in early winter, associated with the East Atlantic pattern. The predictability is strongly tied to the ENSO teleconnection to the North Atlantic, though the systems' response to ENSO is systematically too weak. The hindcasts of the East Atlantic index exhibit a substantial signal-to-noise errors, with the systems' predicted signal generally being smaller than would be expected for the observed level of skill, though there is substantial spread across systems. The signal-to-noise errors are found to be strongly linked to the strength of the ENSO teleconnection in the systems, those with a weaker teleconnection exhibit a larger signal-to-noise problem. The dependency on modelled ENSO teleconnection strength closely follows a simple scaling relationship derived from a toy model. Further analysis reveals that the strength of the ENSO teleconnection in the systems is linked to climatological biases in the behaviour of the North Atlantic jet. 

How to cite: O'Reilly, C.: Signal-to-noise errors in early winter Euro-Atlantic predictions linked to weak ENSO teleconnections and pervasive North Atlantic jet biases, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18821, https://doi.org/10.5194/egusphere-egu25-18821, 2025.

EGU25-21570 | ECS | Posters on site | CL4.6

Predicting climate indicators at the decadal scale using a hybrid prediction system: application to SUEZ water management plans over France 

Joanne Couallier, Ramdane Alkama, Charlotte Sakarovitch, and Didier Swingedouw

As climate change reshapes hydrological cycles, workers in water management face unprecedented challenges in ensuring resource availability, mitigating flood risks, and maintaining resilient infrastructure. Nowadays, water utilities and authorities rely on long-term climate projections to plan for challenges extending through the end of the century. However, critical gaps persist in actionable information for shorter timescales, such as the decadal scale, which better aligns with political and operational decision-making. In this context, decadal climate predictions can be pivotal to address the needs of the water management sector and develop efficient climate services. However, their added values as compared to projections remained limited up to now.
To better understand user requirements, we collaborate with various teams from SUEZ, a company specializing in water management. Through interviews, we have identified the demand for specific indicators based on climate variables (e.g., precipitation, temperature) and corresponding spatio-temporal scales. Building on this understanding, we also develop in IPSL-EPOC decadal prediction team a new hybrid approach to improve our forecasts. This approach includes identifying a climate index (e.g., NAO, WEPA) derived from Sea Level Pressure (SLP) that correlates with the climate variable of interest. Using all the available decadal climate predictions from the DCPP project, we evaluate the predictability of this index, which is usually high for NAO and WEPA. This index is then employed to subsample a few of member CMIP6 climate projections that are in phase with the prediction of the DCPP ensemble. This latter step allows to inflate the amplitude of the predictable signal, resolving the limitation coming from the signal-to-noise paradox. It is also allowing to perform a proper statistical downscaling, used to refine these forecasts, ensuring their usability for identified needs. The resulting forecasts are designed to integrate seamlessly into SUEZ’s water sector models.
Preliminary work has identified diverse parameters of interest for water management, such as daily precipitation (resource availability forecasting), extreme precipitation events at fine temporal resolution (Combined Sewer Overflows modeling), and the number of very cold or very hot days (linked to risks of water mains and service lines failures, respectively). Early findings also suggest that, for the average precipitation over France, the WEPA index exhibits the largest correlations, unlike the NAO, which has greater influence for other European regions. The production of forecasts is currently underway, and their performance regarding the initially identified parameters will be presented.

How to cite: Couallier, J., Alkama, R., Sakarovitch, C., and Swingedouw, D.: Predicting climate indicators at the decadal scale using a hybrid prediction system: application to SUEZ water management plans over France, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21570, https://doi.org/10.5194/egusphere-egu25-21570, 2025.

EGU25-1679 | ECS | Orals | AS1.1

Effect of boundary layer low-level jet on fog fast spatial propagation 

Shuqi Yan, Hongbin Wang, Xiaohui Liu, Fan Zu, and Duanyang Liu

The spatiotemporal variation of fog reflects the complex interactions among fog, boundary layer thermodynamics and synoptic systems. Previous studies revealed that fog can present fast spatial propagation feature and attribute it to boundary layer low-level jet (BLLJ), but the effect of BLLJ on fog propagation is not quantitatively understood. Here we analyze a large-scale fog event in Jiangsu, China from 20 to 21 January 2020. Satellite retrievals show that fog propagates from southeast coastal area to northwest inland with the speed of 9.6 m/s, which is three times larger than the ground wind speeds. The ground meteorologies are insufficient to explain the fog fast propagation, which is further investigated by WRF simulations. The fog fast propagation could be attributed to the BLLJ occurring between 50 and 500 m, because the wind speeds (10 m/s) and directions (southeast) of BLLJ core are consistent with fog propagation. Through sensitive experiments and process analysis, three possible mechanisms of BLLJ are revealed: 1) The abundant oceanic moisture is transported inland, increasing the humidity of boundary layer and promoting condensation; 2) The oceanic warm air is transported inland, enhancing the inversion layer and favouring moisture accumulation; 3) The moisture advection probably promotes low stratus formation, and later it subsides to be ground fog by turbulent mixing of fog droplets. The fog propagation speed would decrease notably by 6.4m/s (66%) in the model if the BLLJ-related moisture and warm advections are turned off.

How to cite: Yan, S., Wang, H., Liu, X., Zu, F., and Liu, D.: Effect of boundary layer low-level jet on fog fast spatial propagation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1679, https://doi.org/10.5194/egusphere-egu25-1679, 2025.

During 29th July to 1st August in 2023, a persistent heavy rainfall event (“23·7” event) hit North China causing severe floods, enormous infrastructure damage and large economy loss. Observational analysis shows that the extremely large accumulation of precipitation and long duration of this event are closely related to a slowly moving landfall typhoon “Dusuari” over North China due to the blocking effect of an anomalous high over the mid- and high-latitude Asia. The anomalous southeasterly flow induced by the typhoon “Dusuari” and another typhoon “Kanu” over the East China Sea jointly built a highly efficient channel of water vapor supplying from southern oceans towards North China. A water vapor budget analysis indicates that precipitation of this event is mainly caused by dynamic process involving strong ascending motion. Accompanying strong water vapor transportation and convergence over North China, large amount of latent heat is released in the middle and lower troposphere. The physical mechanisms of heavy rainfall-induced diabatic heating in maintaining the precipitation over North China is further investigated using statistics analysis and numerical experiments. On one hand, the latent heating released by heavy rainfall induces significant uplifting flows which causes more precipitation. On the other hand, the heavy rainfall-induced diabatic heating contributes to enhancement of the westward extension of high-pressure dam around the Mongolian Plateau through a regional meridional circulation. This strengthened high pressure dam sustained the cyclonic circulation of “Dusuari” over North China, leading to continuous heavy rainfall there.

How to cite: Zhao, W.: Mechanisms of persistent extreme rainfall event in North China, July 2023: Role of atmospheric diabatic heating, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1762, https://doi.org/10.5194/egusphere-egu25-1762, 2025.

EGU25-1763 | ECS | Orals | AS1.1

Wind profile warning characteristics of short-term heavy rain during the Meiyu season 

Jingyu Wang, Chunguang Cui, Xiaokang Wang, and Xiaofang Wang

This study examines the spatial and temporal distributions of short-term heavy rain (SHR) in the middle Yangtze River basin (MYRB) in the summers of the past decade. SHR events are most frequent during the annual Meiyu periods, significantly contributing to total precipitation. Additionally, these events generally last longer and tend to peak at night. The occurrence of SHR events decrease from southeast to northwest, influenced by the monsoonal flow and the small-scale terrain. Moisture convergence prior to Meiyu SHR events is predominantly influenced by both southerly and easterly winds below 700 hPa. Frequent low-level jets and quasi-steady cyclonic circulation lead to strong southerly winds prevailing over the eastern MYRB, while weaker easterly winds dominate in the west. Wind profiles derived from wind profile radar products illustrate the preceding changes in wind speed, wind directions, and vertical wind shear below 4 km above ground level (AGL), as well as the timing of these changes. In the plain area of southeastern MYRB, accelerated southwesterlies are observed 3 to 4 hours before SHR events, accompanied by an intensification of southerly winds near the boundary layer top 2 hours prior. Within the hour leading up to the SHR events, wind speeds sharply rise to their peak. In front of the mountains in west MYRB, southwesterlies strengthen 5 hours in advance but then weaken as they shift to northerlies. Just before the SHR events, however, reinforced northerlies occur near the surface. In the mountainous region of western MYRB, while changes in wind speed are minimal due to topographic blocking, the frequency of southeasterly components below 2 km AGL significantly increases 4 hours before SHR events. The preceding timing of significant vertical wind shear coincides with the increase in wind speed and the change in wind direction. Understanding the detailed characteristics of wind profiles preceding the SHR events during the Meiyu seasons can provide valuable insights for localized severe weather early warning systems. 

How to cite: Wang, J., Cui, C., Wang, X., and Wang, X.: Wind profile warning characteristics of short-term heavy rain during the Meiyu season, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1763, https://doi.org/10.5194/egusphere-egu25-1763, 2025.

Convective clouds during the Mei-yu season contribute significantly to the total rainfall and related disasters over the middle and lower reaches of the Yangtze River in China. Studying the effects of aerosols on convective clouds is of great importance to weather and climate research. However, there are still many open questions to address. This study investigated the effects of aerosol on convections with different cloud geometrical thickness (CGT) bins during the 2018 Mei-yu season, which lasted for 17 days from 18 June to 5 July. Contrasting aerosol effects on shallow and deep convective clouds were revealed by means of anthropogenic aerosol experiments in the Weather Research and Forecasting model with Chemistry (WRF-Chem). Specifically, increased anthropogenic aerosols lead to a 9% reduction in total rainfall and a 7.17% decrease in convection occurrences during the Mei-yu season. After adopting a methodology that stratifies the convective clouds by fixing the CGT, we found that increasing aerosols suppress shallow convections with CGT less than 4 km and invigorate deep convections with CGT greater than 4 km. Increased aerosols enhance the scattering of shortwave radiation, resulting in cooling of the surface air and increasing the stability of the regional lower atmosphere, potentially suppressing shallow convection. Meanwhile, in deep convection, with its stronger updraft and more latent heat, convective invigoration occurs under polluted conditions due to the aerosol-related microphysical and dynamical responses. Considering the high-humidity environment during the Mei-yu season, additional relative humidity tests show that the competing aerosol effects come from convective core invigoration and convective periphery processes which enhance evaporation and dissipation, demonstrating relative humidity is a critical factor in maintaining the net aerosol effects on convections. These results contribute to a better understanding of the effects of anthropogenic aerosols on convections during the Mei-yu season and the competing effects of aerosols depending on the ambient environmental conditions.

How to cite: liu, L.: Contrasting aerosol effects on shallow and deep convections during the Mei-yu season in China , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1775, https://doi.org/10.5194/egusphere-egu25-1775, 2025.

The present study assesses the simulated precipitation and cloud properties using three microphysics schemes (Morrison, Thompson, and MY) implemented in the Weather Research and Forecasting model. The precipitation, differential reflectivity (ZDR), specific differential phase (KDP) and mass-weighted mean diameter of raindrops (Dm) are compared with measurements from a heavy rainfall event that occurred on 27 June 2020 during the Integrative Monsoon Frontal Rainfall Experiment (IMFRE). The results indicate that all three microphysics schemes generally capture the characteristics of rainfall, ZDR, KDP, and Dm, but tend to overestimate their intensity. To enhance the model performance, adjustments are made based on the MY scheme, which exhibited the best performance. Specifically, the overall coalescence and collision parameter (Ec) are reduced, which effectively decreases Dm and makes it more consistent with observations. Generally, reducing Ec leads to an increase in the simulated content (Qr) and number concentration (Nr) of raindrops across most time steps and altitudes. With a smaller Ec, the impact of microphysical processes on Nr and Qr varies with time and altitude. Generally, the autoconversion of droplets to raindrops primarily contributes to Nr, while the accretion of cloud droplets by raindrops plays a more significant role in increasing Qr. In this study, it is emphasized that even the precipitation characteristics could be adequately reproduced, accurately simulating microphysical characteristics remains challenging and it still needs adjustments in the most physically based parameterizations to achieve more accurate simulation.

How to cite: Zhou, Z.: An evaluation and improvement of microphysical parameterization for a heavy rainfall process in Meiyu season, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1816, https://doi.org/10.5194/egusphere-egu25-1816, 2025.

EGU25-1939 | Orals | AS1.1

Stochastic Galerkin method for cloud simulation 

Alina Chertock

In this talk, we consider a mathematical model of cloud physics that consists of the Navier-Stokes equations coupled with the cloud evolution equations for water vapor, cloud water, and rain. In this model, the Navier-Stokes equations describe weakly compressible flows with viscous and heat conductivity effects, while microscale cloud physics is modeled by the system of advection-diffusion-reaction equations. We aim to explicitly describe the evolution of uncertainties arising from unknown input data, such as model parameters and initial or boundary conditions. The developed stochastic Galerkin method combines the space-time approximation obtained by a suitable finite volume method with a spectral-type approximation based on the generalized polynomial chaos expansion in the stochastic space. The resulting numerical scheme yields a second-order accurate approximation in both space and time and exponential convergence in the stochastic space. Our numerical results demonstrate the reliability and robustness of the stochastic Galerkin method. We also use the proposed method to study the behavior of clouds in certain perturbed scenarios, for example, the ones leading to changes in macroscopic cloud patterns as a shift from hexagonal to rectangular structures.

How to cite: Chertock, A.: Stochastic Galerkin method for cloud simulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1939, https://doi.org/10.5194/egusphere-egu25-1939, 2025.

EGU25-2024 | Posters on site | AS1.1

Analysis and research on the impact of terrain on the "23.7" extremely heavy rainstorm 

xiaoyu huang, zhenzhen wu, feng xue, and chenghao fu

From 08:00 on July 29 to 08:00 on August 2, 2023, under the influence of typhoon "Dussuri", an extremely heavy rainstorm process occurs in Hebei and Beijing. The precipitation in some areas of the windward slope of Taihang Mountains exceeds 250mm, and in some areas it exceeds 500mm. The distribution of heavy precipitation is basically consistent with the terrain of the windward slope. Using the 6-minute radar retrieved wind field network data developed by the CMA (China meteorological administration) Meteorological Observation Center for analysis, it is found that from 13:00 on July 29th to 20:00 on August 1st, a southeast-oriented ultra-low-level jet greater than 12 m/s was maintained in the 925-hPa field over Hebei and Beijing. The angle between the jet and the Taihang Mountains is almost 90°, and at the same time, a 850-hPa typhoon trough stays on the windward slope for a long time, resulting in stable and less movement of heavy precipitation echoes. This series of factors together led to the occurrence of the extremely heavy rainstorm process. Using the ERA5 hourly reanalysis data as the initial field and based on the WRF4.5 model, a sensitivity test is conducted on this process using three-layer bidirectional nesting (grid spacing of 9km, 3km, and 1km, respectively). The experiment reduces the Yanshan and Taihang Mountains to half of their original heights and 50 meters, respectively (equivalent to the altitude of Beijing). The experimental results indicate that: (1) Precipitation impact: Due to the easterly winds brought by typhoons, the eastern side of Taihang Mountains is on the windward slope, which has a significant impact on precipitation. When the height of Taihang Mountains decreases, the precipitation intensity significantly weakens; When the terrain height drops to 50m, the precipitation location is biased to the west compared to the actual situation. (2) The experiment showed that the blocking effect of Taihang Mountains formed mesoscale low vortex and convergence line on the windward slope. When the height of Taihang Mountains drops to half of its original height or only 50 meters, the mesoscale low vortex and convergence line move westward to Shaanxi Province. (3) The vertical profile analysis along the east-west direction of Taihang Mountains shows strong upward movement in the windward slope area, with positive vorticity in the lower level and negative vorticity in the upper level. When the height of Taihang Mountains decreases, the upward movement significantly weakens, and the positive and negative vorticity weakens until it disappears, indicating that the dynamic effect of terrain has a significant impact on precipitation processes. (4) The Yanshan Mountains are oriented east-west, and parallel to the environmental winds. Therefore, when its height decreases, its impact on physical quantities such as precipitation, wind field, vertical velocity, and vorticity is relatively small.

Key words: terrain, "23.7" extremely heavy rainstorm, analysis

How to cite: huang, X., wu, Z., xue, F., and fu, C.: Analysis and research on the impact of terrain on the "23.7" extremely heavy rainstorm, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2024, https://doi.org/10.5194/egusphere-egu25-2024, 2025.

EGU25-2044 | Orals | AS1.1

A New Method for Calculating Highway Blocking due to High Impact Weather Conditions 

Duanyang Liu, Tian Jing, Mingyue Yan, and Ismail Gultepe

 Fog, rain, snow, and icing are the high-impact weather events often lead to the highway blockings, which in turn causes serious economic and human losses. At present, there is no clear calculation method for the severity of highway blocking which is related to highway load degree and economic losses. Therefore, there is an urgent need to propose a method for assessing the economic losses caused by high-impact weather events that lead to highway blockages, in order to facilitate the management and control of highways and the evaluation of economic losses. The goal of this work is to develop a method to be used to assess the high impact weather (HIW) effects on the highway blocking. Based on the K-means cluster analysis and the CRITIC (Criteria Importance through Intercriteria Correlation) weight assignment method, we analysed the highway blocking events occurred in Chinese provinces in 2020. Through cluster analysis, a new method of severity levels of highway blocking is developed to distinguish the severity into five levels. The severity levels of highway blocking due to high-impact weather are evaluated for all weather types. As a part of calculating the degree of highway blocking, the highway load in each province is evaluated. The economic losses caused by dense fog are specifically assessed for the entire country.

How to cite: Liu, D., Jing, T., Yan, M., and Gultepe, I.: A New Method for Calculating Highway Blocking due to High Impact Weather Conditions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2044, https://doi.org/10.5194/egusphere-egu25-2044, 2025.

I will introduce a flux globalization-based well-balanced path-conservative central-upwind scheme on Cartesian meshes for the two-dimensional (2-D) two-layer thermal rotating shallow water equations. The scheme is well-balanced in the sense that it can exactly preserve a variety of physically relevant steady states. In the 2-D case, preserving general "moving-water" steady states is difficult, and to the best of our knowledge, none of existing schemes can achieve this ultimate goal. The proposed scheme can exactly preserve the 𝑥- and 𝑦-directional jets in the rotational frame as well as certain genuinely 2-D equilibria. Numerical experiments demonstrate the performance of the proposed scheme in computationally non-trivial situations: in the presence of shocks, dry areas, non-trivial topographies, including discontinuous ones, and in the case of hyperbolicity loss. The scheme works equally well in both the 𝑓-plane and beta-plane frameworks.

How to cite: Kurganov, A., Cao, Y., Liu, Y., and Zeitlin, V.: Flux Globalization-Based Well-Balanced Path-Conservative Central-Upwind Scheme for Two-Dimensional Two-Layer Thermal Rotating Shallow Water Equations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2053, https://doi.org/10.5194/egusphere-egu25-2053, 2025.

EGU25-2224 | ECS | Posters on site | AS1.1

Interpretable ultivariate scoring rules based on aggregation and transformation 

Romain Pic, Clément Dombry, Philippe Naveau, and Maxime Taillardat

Proper scoring rules are an essential tool to assess the predictive performance of probabilistic forecasts. However, propriety alone does not ensure an informative characterization of predictive performance and it is recommended to compare forecasts using multiple scoring rules. With that in mind, interpretable scoring rules providing complementary information are necessary. We formalize a framework based on aggregation and transformation to build interpretable multivariate proper scoring rules. Aggregation-and-transformation-based scoring rules can target application-specific features of probabilistic forecasts, which improves the characterization of the predictive performance. This framework is illustrated through examples taken from the weather forecasting literature and numerical experiments are used to showcase its benefits in a controlled setting. Additionally, the framework is tested on real-world data of postprocessed wind speed forecasts over central Europe. In particular, we show that it can help bridge the gap between proper scoring rules and spatial verification tools.

How to cite: Pic, R., Dombry, C., Naveau, P., and Taillardat, M.: Interpretable ultivariate scoring rules based on aggregation and transformation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2224, https://doi.org/10.5194/egusphere-egu25-2224, 2025.

EGU25-2650 | ECS | Orals | AS1.1

Constraining Future Changes in Extreme Precipitation Using Typical Synoptic Patterns 

Yang Hu, Yanluan Lin, Jiawei Bao, and Yi Deng

The middle and lower reaches of the Yangtze River (MLYR) suffers from extreme precipitation (EP) during summer, which has a huge impact on human society and ecosystem. However, the large spreads among climate models hinder their application in future risk assessment. In this work, four typical synoptic patterns (SPs) triggering EP over MLYR are identified based on the clustering algorithm. And we found a significant linear correlation between the CMIP6 (sixth phase of Coupled Model Intercomparison Project) models’ ability to reproduce the observed typical SPs in present-day climate and the projected future changes of EP over MLYR. Then we proposed an emergent constraint method for EP projections based on this linear correlation and the observed SPs. Using this method, the model spread is evidently narrowed, which increases the credibility of projected future EP changes.

How to cite: Hu, Y., Lin, Y., Bao, J., and Deng, Y.: Constraining Future Changes in Extreme Precipitation Using Typical Synoptic Patterns, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2650, https://doi.org/10.5194/egusphere-egu25-2650, 2025.

From July 29 to August 1, 2023, extreme heavy rainfall occurred in the Chinese HUABEI region. Heavy rainstorm occurred in the most areas of Beijing, Tianjin and Hebei province. The daily precipitation of 14 national meteorological observatories  exceeded the historical extreme value. The process intensity exceeded the three extreme rainstorm processes in the history of HUABEI region. Studying the causes of extreme heavy precipitation in HUABEI and evaluating the predictive performance of the model for extreme heavy precipitation is beneficial for improving the application and forecasting ability of the model. This article analyzes the weather scale characteristics and anomalies of this precipitation process from factors such as height field, wind field, divergence field, vorticity field, and water vapor. The dynamic and thermal structure of the vortex and the cause of the upper level continental high  are analyzed using the method of cyclone phase space map and full type vorticity equation. Finally, the predictive ability of the model for extreme precipitation is tested. The following main conclusions have been drawn:(1) The precipitation process is divided into two stages. Before the 31st, it was caused by the residual vortex circulation of the "Dussuri", with strong precipitation intensity and range. After the 31st, it was formed by the convergence of the easterly jet on the west side of the subtropical high pressure and its interaction with the terrain. Precipitation was mainly concentrated in the northern part of China, with weaker rainfall intensity compared to the previous period.(2) The key impact systems of this process are the 200hPa high trough and continental high pressure, the 500hPa blocking high pressure, and the residual circulation of the low-level "Dussuri". The divergence in front of the 200hPa high altitude trough is beneficial for maintaining upward movement in the North China region; At 500hPa, there is a blocking high pressure in the northern and eastern parts of North China, which is conducive to the maintenance of low-level vortex systems. The "Dussuri" convergence circulation is the triggering system of the process.(3) The water vapor conditions during this process were exceptionally good, mainly consisting of three water vapor transport paths: the southerly water vapor transport of the South China Sea monsoon, the eastward water vapor transport of the residual circulation of "Dussuri", and the southeast water vapor transport path of typhoon "Kanu".(4) During the northward movement, the residual vortex of the Dussuri maintains a quasi symmetric and warm center structure, with weak cold advection in the upper level of the vortex on the 30th.(5) The uneven vertical distribution of condensation latent heat heating generates negative vorticity in the upper troposphere, ensuring the stable maintenance of continental high pressure.(6) In global model forecasting, the CMA model cannot report a blocking high pressure above 96 hours of time. The EC deterministic model can predict heavy precipitation processes within a 120 hour time frame, and the ensemble forecast can have a predictable time frame of up to 7 days.

How to cite: guan, Y.: Analysis and Model Verification of Extreme rainfall Processes in Huabei of China in 2023, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2697, https://doi.org/10.5194/egusphere-egu25-2697, 2025.

This article introduces the five-year research plan of the project and the preliminary progress made over the past two years: 1. Implemented tracking observation experiments on the Mei-Yu frontal extreme precipitation associated in the middle and lower reaches of the Yangtze River for the years 2023 and 2024; 2. Investigated the triggering and maintenance mechanisms of extreme precipitation related to multi-scale interactions and associated thermodynamic conditions; 3. Conducted studies on the microphysical structure and evolution simulation of extreme precipitation. To be specific, the mechanism of low-level jet formation is analyzed during the rainy season in the Yangtze River Basin in 2024.

How to cite: Cui, C. and Wang, B.: Preliminary results on the Mei-Yu Frontal Heavy Rainfall Tracking Observation Experiment and Related Studies, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3219, https://doi.org/10.5194/egusphere-egu25-3219, 2025.

In this study, the microphysical characteristics of summer and winter liquid rainfall are analyzed by 4 Parsivel sites in Hubei Province in the middle reaches of the Yangtze River during 2015-2018. The possible reasons for summer and winter DSD differences are also discussed. The main conclusions are summarized as follows:

(1) Hubei Province is dominated by stratified rainfall in winter, while summer includes convective, stratified, and mixed rainfall. Compared with winter, the average rain rate and Dm in summer are larger, the number concentration Nw is relatively smaller, while difference between δM is very small. The PDF distribution of Dm peak value are about 1.0 mm both in summer and winter, and the Dm data is skewed to the right while the Nw show the opposite.

(2) With increasing rain rate, the Dm increases in both summer and winter. For rain rate R < 2 mm h-1, there are larger Dm and smaller Nw in summer than that in winter, while for the rain rete R > 2 mm h-1 shows the opposite.

(3) There are differences in the μ-λ and Z-R relationships between summer and winter in the middle reaches of the Yangtze River. The relationships also different from those in the lower reaches of the Yangtze River.

(4) The middle reaches of the Yangtze River are mainly influenced by the warm and humid air transport originates in the subtropical South Indian Ocean. In summer, the convective rainfall raindrops grow by collision–coalescence mechanism, and the break-up mechanism also plays an important role which makes smaller diameter. The ice particles could grow sufficiently and fall to the ground with enough time by the accretion mechanism in winter.

In summary, this study gives an insight into the seasonal characteristics of rainfall microphysics in summer and winter, which are very useful for radar QPE and numerical forecasting models modify in the middle reaches of the Yangtze River. However, due to the limitation of observation data, more types of observation data and numerical models simulation should be included to understand the mechanism of the microphysical processes for future reach.

How to cite: Wang, B. and Fu, Z.: The seasonal characteristics of summer and winter raindrops size distribution in Central China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3232, https://doi.org/10.5194/egusphere-egu25-3232, 2025.

EGU25-3272 | Orals | AS1.1

Climate change will increase aircraft take-off distances and reduce payloads, but by how much? 

Jonny Williams, Paul Williams, Federica Guerrini, and Marco Venturini

Climate model output at 30 European airports (including 25 of the busiest) is used to investigate summer take-off distance required – TODR – and maximum take-off mass – MTOM – and how they may change in the future. We compare data from 2035–2064 to a historical baseline of 1985–2014 using three future forcing scenarios which represent low (SSP1-2.7), medium (SSP3-7.0), and high (SSP5-8.5) future emissions trajectories defined by the widely used Shared Socioeconomic Pathways, SSPs.

This work presents data for the A320 aircraft manufactured by Airbus but the calculation framework is widely applicable to any similar fixed-wing aircraft and uses entirely open-access input data.

We use 10 models from the 6th Coupled Model Intercomparison Project (CMIP6) which have a range of equilibrium climate sensitivity values; a measure of the amount of global warming they give for a doubling of carbon dioxide concentrations.

We use a numerical scheme which considers the resultant forces on an aircraft in the runway acceleration phase of its take-off and show that 30-year average values of TODR could increase by up to 100 m by mid-century. There is, however, significant variability since daily data is used throughout.

We quantify the changing probability distribution of TODR using kernel density estimation and illustrate this using an example showing how increases in extreme daily maximum temperature could alter distributions of TODR.

Additionally, we project that the 99th percentile (a one in a hundred day event) of the TODR from 1985-2014 may by exceeded on as many as half the summer days for some sites in the future.

Four of the airports studied (Chios, Pantelleria, San Sebastian and Rome Ciampino) have runway lengths which are shorter than the TODR when the aircraft is carrying its maximum payload. This means that the weight they carry must be reduced to fulfil safety constraints, which will only become more stringent as temperatures increase further. Relative to the mean weight-restriction amount for the historical period, we find that the number of passengers may have to be reduced by up to 10-12 passengers per flight, again accompanied by a significantly increased chance of exceeding extreme historical values.

How to cite: Williams, J., Williams, P., Guerrini, F., and Venturini, M.: Climate change will increase aircraft take-off distances and reduce payloads, but by how much?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3272, https://doi.org/10.5194/egusphere-egu25-3272, 2025.

EGU25-3417 | Posters on site | AS1.1

Evolution and Cause Analysis of a Heavy Precipitation Process of Meiyu Along Yangtze River 

Houfu Zhou, Nan Ge, and Wen Qi

Based on the observational and forecast datasets from precipitation merging product, radiosonde, Doppler radar, wind profiler radar and ECMWF product, the evolution and causes of the heavy precipitation process of Meiyu in the middle and lower reaches of the Yangtze River in China from June 21 to 22, 2024 were analyzed. The results show as the followings. (1) The heavy precipitation was mainly distributed in the northern part of Hunan Province, the southeastern part of Hubei Province and the western part of Anhui Province, with the main period from 15:00 on June 21 to 15:00 on June 22, especially in the early morning of June 22. The rain belt was located to the north of the subtropical high, in the north of the low-level jet, and at the front side of the moving trough line. (2) The K index exceeded 38℃ in all areas, and the CAPE before and after this heavy precipitation process was over 800 J/kg and less than 100 J/kg, respectively, indicating the evolution characteristics of unstable atmospheric stratification as well as the energy accumulation and release. (3) In the early stage of this process, the surface high temperature was distributed to the south of Wuhan, and the near-surface convergence line extended from the eastern part of Henan Province to the central part of Hubei Province. In the middle stage of this process, the convergence line moved eastward. In the later stage of this process, there was a significant cold pool over the land surface along the Yangtze River. The near-surface high temperature and convergence line were the triggering mechanisms of the heavy precipitation, while the cold pool led to the gradual weakening of the precipitation. (4) The water vapor flux was mainly located in the northern part of Hunan Province, the eastern part of Hubei Province as well as the southern part of Anhui Province, and gradually moved eastward. The flux values in the middle and lower layers were relatively high in the early morning of June 22. There were two water vapor transport belts in the lower layer, corresponding to different heavy precipitation centers. (5) The approximately east-west oriented echo band moved from west to east through the forms of merging, strengthening and dissipating. The south side of the echo band was the mesoscale linear or hook-shaped strong echo accompanied by high echo top and strong VIL. The meso-β scale convective system was composed of several meso-γ scale convective cells, and the meso-γ scale convective cells caused strong cumulative precipitation through the ‘train effect’.

How to cite: Zhou, H., Ge, N., and Qi, W.: Evolution and Cause Analysis of a Heavy Precipitation Process of Meiyu Along Yangtze River, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3417, https://doi.org/10.5194/egusphere-egu25-3417, 2025.

EGU25-3842 | Posters on site | AS1.1

 IAGOS estimates of climate-process costs for trans-Atlantic flights 

Corwin Wright

IAGOS, or the In-service Aircraft for a Global Observing System project, is a European Infrastructure project consisting of scientific measurement packages attached to commercial aircraft. Operating since 1994, this programme provides a unique long-timeseries dataset of flight data across the globe, with thousands of flights per year providing a strong base for statistical studies.

Here, we use flight times derived from IAGOS metadata to quantify the role of the El Nino - Southern Oscillation (ENSO), the Quasi-Biennial Oscillation, the solar cycle and the North Atlantic Oscillation (NAO) on trans-Atlantic flight times. We do this both by subsetting the data in various ways and via regression methods. This allows us to statistically assess the effects of these large-scale atmospheric-dynamical processes on trans-Atlantic flight times. We also calculate the additional costs associated with these effects in terms of both carbon dioxide emissions and fuel costs, allowing us to understand how climate processes drive them.

Depending on season and direction of flights, we show that these four climate indices can explain as much as 1/3 of the total variance in trans-Atlantic flight times. At a flight-time level and particularly in winter, the NAO dominates flight times and is the most important factor in one-way fuel costs: flights at peak NAO+ can be as much as 83 minutes longer than the equivalent flight at peak NAO- when crossing the Atlantic. However, at a whole-dataset level, ENSO is shown to be much more important in driving net round-trip costs. We further estimate that the monthly cost of these four climate indices can be as high as 100 kT of additional CO2 or USD 20 million at 2023 flight volumes and fuel prices.

How to cite: Wright, C.:  IAGOS estimates of climate-process costs for trans-Atlantic flights, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3842, https://doi.org/10.5194/egusphere-egu25-3842, 2025.

The MicroWave Humidity Sounder II (MWHS II) is a cross-track microwave sounder flying on FengYun (FY)-3C satellite. It has 15 channels ranging from 89.0 to 191.0 GHz, eight (channels 2-9) of which are located near 118.75 GHz along an oxygen absorption line, five (channels 11-15) of which are located near 183.31 GHz water vapor absorption line and the remaining two channels 1 and 10 are two window channels centered at 89.0 and 150.0 GHz. A new precipitation detection algorithm for 118GHz channels was developed based on the radiation characters of the double O2 absorption bands (118 and 50-60 GHz). Since both of the 118 GHz and 50-60 GHz oxygen absorption bands are sensitive to atmospheric temperature, the radiation observed in the two bands has a specific inherent constraint relationship under the clear-sky conditions. However, the frequencies of 118 GHz channels are approximately twice that of the 50-60 GHz channels, and the two bands have different absorption and scattering characteristics for atmospheric hydrometeors. The radiance transfer mode VDISORT was used to simulate the sensitivity of the 118 GHz and 50-60 GHz channels to five kinds of hydrometeors (cloud water, rainwater, ice, snow, and graupel) in the cloud atmosphere. The results show that the 50-60 GHz channels are more sensitive to rainwater, and the 118 GHz channels are more sensitive to the other four types of hydrometeors. Therefore, the inherent constraint of the observational radiance between 118 GHz and 50-60 GHz channels under clear-sky condition is no longer valid for a cloudy scenario. In this paper, the machine learning system TensorFlow was used to construct a model for predicting the brightness of 118 GHz channels using 50-60 GHz observations under clear-sky conditions, and the accuracy of the prediction model was validated using independent samples. Then this neural network-based predictive model was used for 118 GHz channel precipitation detection. When the difference between actual observed and predicted bright temperature for 118 GHz channel is more massive than three times of the standard deviation of the prediction model, it is thought that the MWHS II observation is contaminated by precipitation or cloud. At last, this new precipitation detection algorithm for 118 GHz was validated by simulated measurements. The results show that both the precipitation detection POD (test probability) and PC (correct rate) for 118 GHz channels are above 90%.

How to cite: Guo, Y.: A precipitation detection algorithm for 118GHz channels based on FY-3C MWHS II and FY-3C MWTS II, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3880, https://doi.org/10.5194/egusphere-egu25-3880, 2025.

EGU25-4138 | ECS | Orals | AS1.1

Methodological Focus on Hyperparameters for Different Rain Nowcasting Models 

Baptiste Guigal, Aymeric Chazottes, Laurent Barthès, Nicolas Viltard, Erwan Le Bouar, Emmanuel Moreau, and Cécile Mallet

Precipitation nowcasting plays an essential role in operational weather forecasting services. Sudden precipitation events have significant socio-economic impacts, including natural disasters like flash floods. This challenge is becoming increasingly critical as climate change alters weather patterns and the frequency of extreme weather events continues to increase.

Over the last decade, radar observations, offering high temporal and spatial resolution, have facilitated the development of machine learning methods for precipitation nowcasting. Once trained, these methods are well suited to processing large datasets with low latency, especially in a real-time context. Recent advances in the field of nowcasting have focused on optimizing model architectures, improving loss functions for imbalanced data, and integrating multivariate inputs, including radar and satellite observations.

This study explores some critical hyperparameters, such as temporal context length, edge effect during training, influence of the output horizons prediction, and convolution kernel size. To do this, we investigate the performance of several models, including both machine learning approaches from different families, in particular SmaAt-Unet, ConvLSTM , and DGMR (trained on UK rains) , as well as non-machine learning methods such as  STEPS. An eleven years consistent radar precipitation dataset covering the Paris region was set up from Météo-France mosaic. Nine years were used for training machine learning models, and two years were reserved to evaluate the models’ performances. To assess the model in different weather conditions, the data set is divided into four groups with distinct characteristics corresponding to various meteorological phenomena. To ensure consistent evaluation, we evaluated the models on the same two-year test dataset, focusing on three criteria, namely: spatial consistency (Pearson correlation coefficient), location accuracy (CSI), and precipitation intensity (MSE).

Our analysis reveals that machine learning models consistently outperform traditional optical flow methods, with notable variations in performance across timescales and rainfall intensities. We also highlight that performance is nearly identical for all models in the presence of stratiform rain, while there are substantial differences in the convective rain group. Additionally, we show that for deep learning models, considering edge effects during training prevents the propagation of inevitable errors and helps avoid the appearance of ghost rain cells at the edges of the map. Furthermore, we show that the size of the kernels of the first layers plays an important role and must be large enough to allow correlation between distant pixels.

Finally, our study provides guidelines for the development of precipitation nowcasting models.

How to cite: Guigal, B., Chazottes, A., Barthès, L., Viltard, N., Le Bouar, E., Moreau, E., and Mallet, C.: Methodological Focus on Hyperparameters for Different Rain Nowcasting Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4138, https://doi.org/10.5194/egusphere-egu25-4138, 2025.

EGU25-5038 | Posters on site | AS1.1

On the Dynamical Core of Aeolus 2.0: An Atmospheric Model Using a Moist-Convective Thermal Rotating Shallow Water Framework 

Masoud Rostami, Stefan Petri, Bijan Fallah, and Farahnaz Fazel-Rastgar

This study introduces Aeolus 2.0[1, 2], a novel multilayer moist-convective Thermal Rotating Shallow Water (mcTRSW) model designed to simulate atmospheric dynamics under various forcings, such as increased radiative or thermal forcing, as well as the effects of latent heat release and radiative transfer on meso- and large-scale dynamics. The model incorporates a novel moist-convective scheme that respects conservation laws, a new bulk aerodynamic scheme for sea surface evaporation and sensible heat flux, and provides a computationally efficient yet physically robust framework, bridging the gap between idealized models and complex general circulation models. Aeolus 2.0 integrates barotropic and baroclinic processes, enabling detailed investigations of phenomena such as zonal wind variability, heatwaves, and seasonal energy fluxes.

The model has already been applied to various atmospheric phenomena, such as simulating the Madden-Julian Oscillation (MJO)[3], large-scale localized extreme heatwaves[4], and atmospheric responses to increased radiative forcing during solstices and equinoxes[1]. In this presentation, we showcase the results of the latter. The findings highlight significant changes in zonal wind velocity and meridional temperature gradients, with notable hemispheric asymmetry. Specifically, increased radiative forcing enhances subtropical westerly jet velocities and mid-latitude temperatures during the solstices, while reducing polar cyclone zonal wind velocities in the affected hemisphere. Poleward eddy heat fluxes were consistently observed across hemispheres, and heatwave intensity and duration were amplified over both land and ocean regions.

References:

[1] Rostami, M., Petri, S., Fallah, B., Fazel-Rastgar, F. (2025). Aeolus 2.0's thermal rotating shallow water model: A new paradigm for simulating extreme heatwaves, westerly jet intensification, and more. Physics of Fluids, 37 (1), 016604. https://doi.org/10.1063/5.0244908.

[2] Rostami, M., Petri, S., Guimaräes, S.O., Fallah, B. (2024). Open-source stand-alone version of atmosphere model Aeolus 2.0 Software. Geoscience Data Journal, 11, 1086–1093. https://doi.org/10.1002/gdj3.249. (Link to Zenodo: https://doi.org/10.5281/zenodo.10054154)

[3] Rostami, M., Zhao, B. & Petri, S. (2022). On the genesis and dynamics of madden–Julian oscillation-like structure formed by equatorial adjustment of localized heating. Quarterly Journal of the Royal Meteorological Society, 148, 3788–3813.  https://doi.org/10.1002/qj.4388.

[4] Rostami, M., Severino, L., Petri, S., & Hariri, S. (2023). Dynamics of localized extreme heatwaves in the mid-latitude atmosphere: A conceptual examination. Atmospheric Science Letters, e1188. https://doi.org/10.1002/asl.1188 .

 

How to cite: Rostami, M., Petri, S., Fallah, B., and Fazel-Rastgar, F.: On the Dynamical Core of Aeolus 2.0: An Atmospheric Model Using a Moist-Convective Thermal Rotating Shallow Water Framework, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5038, https://doi.org/10.5194/egusphere-egu25-5038, 2025.

Based on the brightness temperature observed by the Fengyun-4A satellite, eight hundred mesoscale convective systems (MCSs) are identified in the middle reaches of the Yangtze River Basin during the warm seasons of 2018–2021, and these MCSs are categorized into the quasistationary (QS) type and the outward-moving (OM) type. Afterward, the initiations of the MCSs are backward tracked using a hybrid method of areal overlapping and optical flow. Then, the intensity, evolution and distribution of cloud-to-ground (CG) lightning and radar composite reflectivity (CR) associated with MCSs are explored.

The QS-MCSs primarily occur in July and August and are mainly initiated in the afternoon. The OM-MCSs mostly occur in June and July with two initiation peaks at noon and late night, respectively. The QS-MCSs are mainly initiated in mountainous areas. In contrast, the OM-MCSs are mainly initiated in plain areas. Compared to the OM-MCSs, the QS-MCSs show notable diurnal variation in intensity and develop more rapidly. The geographical distribution of CG lightning associated with MCSs shows that the highest occurrence tends to appear over the transition zone of the Poyang Lake Plain and the surrounding mountains. The CG lightning associated with MCSs features a relative lower proportion of negative CG lightning occurrences. An overall negative correlation between brightness temperature and the peak current of CG lightning is documented with seasonal variations. The advection of ice particles associated from convective cores into nearby stratiform regions caused by relatively stronger mid-to-upper-level winds, may explain the positive correlations in May and September. A time lag of 0–2 h between the CG lightning occurrence peak and the MCS extent maximum is found. As the MCS develops, the proportion of convective clouds decreases, the proportion of nonprecipitating anvil increases, and the proportion of stratiform consistently maintains 50%–60% of the MCS extent, dominating throughout its life span. The main region for stratiform is primarily in the southern part of the MCS, while convective clouds are mainly in the northern part, possibly due to the influence of the Meiyu front.

 

How to cite: Sun, J. and Fu, Y.: The Intensity, Evolution, and Distribution of Cloud-to-Ground Lightning and Radar Reflectivity throughout the Life Cycle of Mesoscale Convective Systems over Southern China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5335, https://doi.org/10.5194/egusphere-egu25-5335, 2025.

EGU25-5755 | ECS | Orals | AS1.1

Informing the Unification of a Single Cloud Fraction Scheme in the Met Office’s Unified Model   

Francesca Cottrell, Paul Barrett, Steven Abel, Michael Whitall, Keith Williams, and Paul Field

The choice of cloud fraction parametrization scheme in weather and climate models significantly influences model performance. Currently in the Met Office’s Unified Model (UM), two different approaches are used to represent sub-grid clouds: a prognostic scheme in the global atmosphere and land (GAL) configuration, and a diagnostic scheme in the regional atmosphere and land (RAL) configuration.  Historically, prognostic schemes have performed better at climate resolutions where memory is important, whilst diagnostic schemes have been sufficient for higher resolution numerical weather prediction (NWP). Due to recent increases in computational power, both climate simulations and NWP are being run at higher resolutions. This blurs the boundary between the two configurations, and it would therefore be beneficial to unify a single large-scale cloud fraction scheme which works seamlessly across all resolutions. 

A framework for testing candidate cloud fraction schemes has been developed, using high resolution (300m grid spacing) simulations. This grid spacing was chosen as previous comparisons of the UM with observational data show a cloud fraction scheme is required, however most deep convection will be resolved at this resolution and so there is no need for a convection scheme.  

We investigate four different cloud fraction schemes: Smith (diagnostic), Bi-Modal (diagnostic), PC2 (prognostic), and a new hybrid cloud scheme combining PC2 for ice and Bi-Modal for liquid. We also look at two cloud microphysics schemes: Wilson & Ballard (single moment), and Cloud AeroSol Interacting Microphysics (CASIM; double moment).  

Simulations of shallow cumulus and stratocumulus cloud regimes have been performed over a south UK domain for several case study dates. Through comparisons of rainfall rates and storm cell sizes against 1 km radar observations, it’s been demonstrated that all model configurations overpredict the number of small cells even at this high resolution, particularly GAL9 which also hugely overpredicts rainfall rates. Further comparisons against 3D radar composites provide information on timing and morphology errors. In addition, comparisons against the observations from the Wessex UK Summertime Convection Experiment (WesCon) provide further constraints for single-site model output for parameters including liquid water path and cloud-base height. Together, these comparisons will help to identify the configuration that best represents observed cloud at high resolutions, thereby informing the development of a unified physics configuration.   

How to cite: Cottrell, F., Barrett, P., Abel, S., Whitall, M., Williams, K., and Field, P.: Informing the Unification of a Single Cloud Fraction Scheme in the Met Office’s Unified Model  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5755, https://doi.org/10.5194/egusphere-egu25-5755, 2025.

Cloudburst is a new post-processing system at the Met Office, leveraging Amazon Web Services (AWS) to provide a route for easy deployment of post processing pipelines allowing for the generation of replacement data as legacy sources are retired. The focus is primarily on generating diagnostics where consistency across multiple variables is required to provide a coherent weather narrative. Thus far all provided parameters have utilised the Met Office’s global and UK deterministic models but the system is made to be versatile so ensemble forecasts could be used in future.

The diagnostics generated in Cloudburst use code from the open-source IMPROVER (Integrated Model post-PROcessing and VERification) repository, which offers a versatile toolbox of post-processing plugins. By enhancing this toolbox with new plugins and functionalities, we promote the reusability of post-processing components, fostering collaboration between the Blended Probabilistic Forecast team and the Cloudburst team. Any code added to the IMPROVER repository by Cloudburst is made as adaptable as possible so that it could be applied to deterministic forecasts or ensemble members.

In this presentation we will describe the first diagnostic generated within Cloudburst: precipitation type. This diagnostic was required to be consistent with the rain and snow rate so these were also rederived from the precipitation rate. Precipitation type, along with rain and snow rates, have now been operationalised and the data sent downstream for customers.

How to cite: Spelman, M.: Cloudburst: A Platform for Running Post-Processing Workflows at the Met Office, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5870, https://doi.org/10.5194/egusphere-egu25-5870, 2025.

EGU25-6014 | ECS | Orals | AS1.1

Data-driven dynamic motion field generation for rainfall nowcasting 

Ruben Imhoff, Daniel A. Blázquez Martín, Riccardo Taormina, and Marc Schleiss

Rainfall nowcasting algorithms rely primarily on extrapolation, where recent radar rainfall observations are projected forward in time based on a motion field that is determined with past data. While additional (stochastic) processes may be incorporated, as is for example done in the pySTEPS models, extrapolation remains the fundamental mechanism. Although the motion field estimates are robust, they assume a steady state in the motion field for the future. This assumption can face significant challenges in maintaining accuracy over time, especially during convective weather events characterized by rapid changes in precipitation patterns and their movement.

In this study, we focus on three objectives: 1) identifying the current errors and uncertainties in the steady-state motion field derivation using pySTEPS, 2) the construction of a dynamic motion field derivation approach using a new deep-learning model, MotioNNet, and 3) the development of ensemble motion fields for MotioNNet. MotioNNet is a U-Net based deep-learning architecture, which uses the past radar images (five in this study) in combination with the estimated static motion field from pySTEPS to estimate the deviation from the provided static motion field per grid cell with increasing lead time. For the ensemble generation in MotioNNet, we tested probabilistic techniques such as SpatialDropout and Monte Carlo dropout.

We trained and tested our model on C-band weather radar data from the Royal Netherlands Meteorological Institute (KNMI), using 10,000 rainfall events. These events were selected to include cases with both intense precipitation and significant motion errors. Our results show that the static motion field approach results in average motion field errors of 1 – 3 km h-1 at the start of the forecast and increases to 4 – 8 km h-1 (on average, and locally sometimes much higher) at a lead time of 90 minutes. The dynamic motion field estimates of MotioNNet improve the motion prediction accuracy by approximately 13%. The improvement is much higher for structured and stable events (up to 45%), but almost negligible for localized thunderstorm events. The results of the ensemble construction in MotioNNet indicate that MotioNNet is capable of adding perturbations in space where most uncertainty takes place, especially for structured and stable events. This is an advantage compared to the spatially uniform approach of pySTEPS. However, the spread of the ensembles is still underestimated, even more so than with pySTEPS, indicating that the uncertainty in the forecast is not yet well represented.

We conclude that the hybrid MotioNNet approach can substitute and enhance parts of the motion field module in pySTEPS. MotioNNet refines initial motion field estimates, rather than replacing them, which leads to a modular approach that fits well in the overall pySTEPS framework. We expect that the dynamic motion field approach from MotioNNet will aid in further enhancing the predictability of (high-intensity) rainfall events for short lead times, especially for structured events where motion errors currently play a role in the forecast error.

How to cite: Imhoff, R., Blázquez Martín, D. A., Taormina, R., and Schleiss, M.: Data-driven dynamic motion field generation for rainfall nowcasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6014, https://doi.org/10.5194/egusphere-egu25-6014, 2025.

EGU25-6937 | ECS | Posters on site | AS1.1

Lead time-dependent postprocessing of 2-meter temperature forecast using a multivariate generative machine learning model  

Sameer Balaji Uttarwar, Jieyu Chen, Sebastian Lerch, and Bruno Majone

The spatiotemporal dependence structure in postprocessed weather forecast variables is essential for reliable hydrological and socio-economic applications. However, in univariate postprocessing, where statistical or advanced machine learning techniques are applied independently in each margin, the multivariate dependence structure present in the raw ensemble forecasts is lost. To restore the disrupted spatial or temporal dependence structure of univariately postprocessed forecasts, copula-based methods are traditionally applied as an additional step that utilizes dependency information from raw ensemble forecasts or historical observations. However, such a two-step framework faces difficulty incorporating exogenous variables to model the dependence structure. To overcome these limitations, a multivariate non-parametric data-driven distributional regression postprocessing technique based on a generative neural network is employed to draw samples directly from multivariate predictive distribution as output [1]. This study focuses on preserving temporal dependency and investigates the performance of a multivariate generative model against two-step approaches to postprocess a 2-meter temperature forecast with a one-month lead time over the Trentino-South Tyrol region in the northeastern Italian Alps. The forecast dataset is a fifth-generation seasonal weather forecast system (SEAS5) generated by the European Centre for Medium-Range Weather Forecasts (ECMWF), which has a 0.125° x 0.125° horizontal grid resolution with 25 ensemble members over a reforecast period from 1981 to 2016. The reference dataset is the high-resolution (250 m x 250 m) gridded observational data over the region. The results are presented using multivariate proper scoring rules (i.e., energy and variogram scores) to measure the overall discrepancy and dependence structure in the postprocessed forecast. The performance analysis reveals that the multivariate generative postprocessing model outperforms the two-step approach over the entire region.

 

References:

[1] Chen, J., Janke, T., Steinke, F. & Lerch, S. Generative Machine Learning Methods for Multivariate Ensemble Postprocessing. Ann. Appl. Stat. 18, 159–183 (2024).

How to cite: Uttarwar, S. B., Chen, J., Lerch, S., and Majone, B.: Lead time-dependent postprocessing of 2-meter temperature forecast using a multivariate generative machine learning model , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6937, https://doi.org/10.5194/egusphere-egu25-6937, 2025.

EGU25-7540 | Posters on site | AS1.1

A Study on Catenary Icing Prediction Method Integrating Physical Modeling and Transformer-Based Deep Learning 

Xiaowei Huai, Wenjun Kang, Bo Li, Jing Luo, Wen Dai, and Rongtao Liu

This paper proposes a novel method for predicting icing on overhead contact lines by integrating physical modeling with Transformer-based deep learning, addressing the limitations of traditional meteorological models in complex weather conditions and terrains. The method combines physical factors such as meteorological data (e.g., temperature, humidity, wind speed) and topographic features to construct a physical model for initial predictions, while leveraging the Transformer model's robust capability in processing time-series data to capture the nonlinear dynamics of the icing process. Experimental results demonstrate that the proposed method significantly outperforms traditional single meteorological models in prediction accuracy across various weather conditions, particularly excelling in extreme weather and complex terrain scenarios. This approach provides reliable technical support for disaster prevention, mitigation, and early warning systems in the transportation sector, offering substantial practical value for engineering applications.

How to cite: Huai, X., Kang, W., Li, B., Luo, J., Dai, W., and Liu, R.: A Study on Catenary Icing Prediction Method Integrating Physical Modeling and Transformer-Based Deep Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7540, https://doi.org/10.5194/egusphere-egu25-7540, 2025.

EGU25-7697 | Posters on site | AS1.1

Characteristics of the Macro- and Micro-Structures of Different Grades of Fog in Jiangsu, China 

Hongbin Wang, Zhiwei Zhang, and Duanyang Liu

Based on the minute-resolution meteorological elements data observed at 70 automatic weather stations in Jiangsu, the second-resolution sounding data of 3 sounding stations and the fog droplet spectrum data of 21 dense fog events, from January 1, 2013 to December 31, 2023, the spatial and temporal distribution, boundary layer structure and microphysical structure characteristics of the fog at different grades in Jiangsu were analyzed. The results show that in recent years, the number of fog hours in Jiangsu are distributed along the Yangtze River and to the north along the Huaihe River. The average annual fogging time at each station is 318.5h, the strong dense fog and extremely dense fog were mainly concentrated along the Huaihe River and its north, accounting for 16.4% of the total fog hours. The probability of occurrence of fog in Jiangsu is the highest at 05:50, and the probability of occurrence of fog in winter, spring, summer and autumn is the highest at 07:10, 05:50, 05:20 and 05:50, respectively. The temperature structure of fog at different grades between 0 and 1500 m has inversion layer, and with the increase of fog intensity, the inversion intensity increases. And the relative humidity is saturated in the lower layer, but with the increase of fog intensity, the relative humidity of upper layer decreases. With the increase of fog intensity, the number of fog drops of different sizes all increase, and the spectrum of fog drops expands obviously when strong dense fog or extremely dense fog occurs.

How to cite: Wang, H., Zhang, Z., and Liu, D.: Characteristics of the Macro- and Micro-Structures of Different Grades of Fog in Jiangsu, China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7697, https://doi.org/10.5194/egusphere-egu25-7697, 2025.

EGU25-7761 | Orals | AS1.1

Future Satellite Observations of the Dynamics and Microphysics of Convection from the NASA Atmosphere Observing System (AOS) 

Scott Braun, Pavlos Kollias, Jie Gong, Yuli Liu, Nobuhiro Takahashi, Takuji Kubota, Helene Brogniez, Thierry Amiot, John Yorks, and Daniel Cecil

Atmospheric convection plays a fundamental role in the vertical redistribution of atmospheric constituents, in driving atmospheric circulation, and in creating severe weather conditions that put life and property at risk. Cloud and precipitation processes in convection and their related release of latent heat are coupled to the rate of vertical air motion in convective updrafts and downdrafts. Observations of vertical air motion in convection have generally been confined to suborbital observations of limited areas and periods of time, but understanding the global distribution of convection is very much needed.

 

The NASA Atmosphere Observing System (AOS) was formulated based on the NASA 2017 Earth Science Decadal Survey to address key objectives tied to aerosols, clouds, convection, and precipitation. As of March 2024, the AOS constellation consists of four individual projects: 1) AOS-Storm, in partnership with JAXA and CNES, flying in a 55° inclined orbit and focusing on convective precipitation, vertical air motions, and convective ice cloud properties; 2) AOS-Sky, a satellite carrying a suite of passive sensors including a multi-angle polarimeter, passive microwave radiometer, and thin ice cloud far infrared imaging radiometer flying in tandem with a CSA-provided spacecraft (called HAWCsat) carrying aerosol and moisture limb imagers; 3) an Italian Space Agency led mission, in partnership with NASA, carrying a multi-frequency elastic backscatter lidar with Raman channels for measurement of aerosol, cloud, ocean, and land properties; and 4) an expected cloud profiling radar to be competed as part of an announcement of opportunity.

 

This talk will focus on the AOS-Storm project consisting of the JAXA Precipitation Measuring Mission (PMM) and the CNES Convective Core Observations through MicrOwave Derivatives in the trOpics (C2OMODO) mission, with NASA providing a spacecraft bus for one of the CNES radiometers and launch of both satellites.  The PMM mission includes a JAXA-provided spacecraft and Ku-band Doppler radar that will provide radar reflectivity across a 255-km swath (similar to TRMM and GPM) and Doppler velocity measurements at nadir in moderate to strong convective systems. The CNES C2OMODO mission consists of two identical passive microwave radiometers (channels near 89, 183, and 325 GHz) flying in tandem with a temporal spacing expected to be in the 30-120 second range. The time-differenced passive microwave brightness temperatures will characterize the rate of change of ice water path and anvil size as well as the vertical flux of ice mass. We will highlight recent simulations of expected performance for measurements of vertical air motions and ice water path in convective clouds.

How to cite: Braun, S., Kollias, P., Gong, J., Liu, Y., Takahashi, N., Kubota, T., Brogniez, H., Amiot, T., Yorks, J., and Cecil, D.: Future Satellite Observations of the Dynamics and Microphysics of Convection from the NASA Atmosphere Observing System (AOS), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7761, https://doi.org/10.5194/egusphere-egu25-7761, 2025.

EGU abstract 2025

NP5.2 EDI: Advances in statistical post-processing, blending, and verification of deterministic and probabilistic forecasts

The challenge of uncertain observations: Probabilistic verification of decadal predictions with high temporal resolution

Verification plays an important role in the evaluation and the development of climate predictions. With new developments in the field and ever larger availability of computational resources, temporal high resolutions become an option. But we often do not make use of the full temporal distribution and much too often we still rely on temporal averages to reduce the dimensionality of the data to make a verification with common metrics manageable. One of the reasons is the challenge how to verify in an understandable manner probabilistic model predictions with probabilistic, uncertain observations.

Tools for probabilistic verification are available, like the Continuous Rank Probability Score (CRPS), but are often defined for perfect observations. Furthermore, many tools are for the wider community hard to comprehend and are as such often not applied. This poses the question on how to verify predictions on the basis of current imperfect usage of metrics within the field and how to communicate prediction skill in general. 

This contribution will address two main approaches and apply it to the comparison between a decadal prediction and the associated projection (historical simulation), with an assimilation simulation as an observational reference. In the first we will ask how to communicate verification results for a wider community. For this we will look at framing the skill as yearly matchups between the two model results. Basing on the Integrated Quadratic Distance each year determines which model result is closer to the observations and the years how often one result was better than the other leads to our verification result. In a second approach it will be discussed to find modifications of some of the most applied metrics in our field, Anomaly Correlation (ACC) and Root-Mean Square (RMS), towards uncertain observations. While these metrics are imperfect, they allow an easy communication for people already applying them. Differences in their interpretation will be discussed, giving us insights about how uncertain observations change our understanding of a good prediction. We address also significance estimation and it will be highlighted why we need to find easy comprehendible approaches to handle uncertain observations in the future.

How to cite: Düsterhus, A.: The challenge of uncertain observations: Probabilistic verification of decadal predictions with high temporal resolution, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8034, https://doi.org/10.5194/egusphere-egu25-8034, 2025.

EGU25-8427 | Orals | AS1.1

A multi-criteria evaluation of the performance of bias correction using Delta Quantile Mapping for simulated precipitation over Germany 

Edgar Espitia, Yanet Díaz Esteban, Moritz Haupt, Muralidhar Adakudlu, Odysseas Vlachopoulos, and Elena Xoplaki

Bias correction techniques are often used as effective and reliable approaches to improve the representation of current and past conditions in climate models. This study aims to evaluate the performance of Quantile Delta Mapping (QDM) as a bias correction method for daily precipitation simulations from climate models: the Icosahedral Nonhydrostatic Model (ICON), the Regional Climate Model COSMO-CLM (CCLM), and the Regional Climate Model (REMO) at a spatial resolution of 3 km over Germany. The dataset consists of historical observations from HYRAS and climate model simulations between 1961 and 1990, split into a calibration period (1961–1980) and an independent validation period (1981–1990). To assess performance, we considered four aspects: 1) sequence of events, 2) distribution of values, 3) spatial structure, and 4) visual inspection of distance metrics, ultimately providing an integrative qualitative ranking across these aspects. Performance metrics included correlation, Nash-Sutcliffe efficiency (NSE), Kling-Gupta efficiency (KGE), and error metrics such as BIAS, mean square error (MSE), and root mean squared error (RMSE). Additional metrics considered were the Kolmogorov-Smirnov (KS) statistic, Perkins Skill Score (Sscore), probability density function (PDF), 80th, 90th, and 95th percentiles, and spatial autocorrelation. As a preliminary assessment of the simulated precipitation from ICON, results show only slight improvements in the time and spatial distribution of precipitation metrics. For example, the KS statistic improved from 0.0314 to 0.0190, while the Sscore improved from 0.0314 to 0.0195 when comparing HYRAS vs. ICON raw and HYRAS vs. ICON bias-corrected using QDM, respectively. Therefore, limited improvement is expected from bias correction when the climate model already performs well, whereas significant improvements can be achieved when the climate models perform only acceptably.

How to cite: Espitia, E., Díaz Esteban, Y., Haupt, M., Adakudlu, M., Vlachopoulos, O., and Xoplaki, E.: A multi-criteria evaluation of the performance of bias correction using Delta Quantile Mapping for simulated precipitation over Germany, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8427, https://doi.org/10.5194/egusphere-egu25-8427, 2025.

EGU25-8449 | Posters on site | AS1.1

The crossing-point quantile: an optimal point-forecast in terms of ROC areas.  

Zied Ben Bouallegue and Maxime Taillardat

A point-forecast is defined as a single-value forecast expressed in the unit of a variable of interest. A deterministic forecast for 2m temperature at Vienna tomorrow is a point-forecast. Point-forecasts are required by some forecast users and for various applications. When an ensemble prediction system is at hand, a point-forecast can take the form of a distribution functional such as the ensemble mean or an ensemble quantile. In this context, we introduce a new type of point-forecast based on the concept of crossing-point forecast (Ben Bouallègue, 2021). We argue that this self-adaptive forecast should be better suited for some users than other point-forecasts. More precisely, we demonstrate that the so-called crossing-point quantile is an optimal forecast in terms of Pierce Skill Score (or equivalently in terms of area under the ROC curve) for any event of interest.  

Ben Bouallègue Z (2021), On the verification of the crossing-point forecast, Tellus A. DOI:10.1080/16000870.2021.1913007 

How to cite: Ben Bouallegue, Z. and Taillardat, M.: The crossing-point quantile: an optimal point-forecast in terms of ROC areas. , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8449, https://doi.org/10.5194/egusphere-egu25-8449, 2025.

EGU25-9468 | Posters on site | AS1.1

Improvements to NWP visibility forecasts using statistical post-processing 

Katharine Hurst and Gavin Evans

Accurate visibility forecasting is essential for aviation, road safety, and maritime operations as well as communicating the weather on a daily basis to the public. Despite advancements in Numerical Weather Prediction (NWP) models, it is well understood in the forecasting community that NWP visibility forecasts are inherently poor, often suffering from calibration issues and systematic biases. In post-processing we can enhance skill, however, it is very difficult to add skill when the input data are particularly poor, so this diagnostic remains a known problem. 

This study explores the application of different parametric and non-parametric statistical post-processing techniques to enhance the accuracy and reliability of visibility forecasts. The chosen method will build upon a new visibility scheme at the Met Office, VERA (Visibility Employing Realistic Aerosol), which uses a more physically realistic representation of the condensation nuclei required to form fog and therefore produces a better distribution of visibility for statistical post-processing to work with. 

The calibration methods included in this study include Quantile Regression Random Forests, Reliability Calibration, Bayesian Additive Regression Trees, and finally Distributional Regression Networks using truncated normal and log normal Continuous Ranked Probability Score loss functions, as well as threshold weighted variants of these loss functions. These methods are tailored, where appropriate, to better support the characteristics of visibility data. 

The methodology is tested on an extensive training dataset from the European Centre for Medium-Range Weather Forecasts (ECMWF), which spans 20 years of reforecasts and several European countries capturing a wide range of visibility conditions, including the rarer low visibility events which are most impactful. 

Initial results demonstrate that Quantile Regression Random Forests post-processed forecasts show a marked reduction in Root Mean Square Error compared to raw NWP outputs, and work is in progress to compare this to other methods. These improvements, so far, highlight the great potential of statistical post-processing in refining visibility predictions and supporting decision-making in weather-sensitive sectors. 

How to cite: Hurst, K. and Evans, G.: Improvements to NWP visibility forecasts using statistical post-processing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9468, https://doi.org/10.5194/egusphere-egu25-9468, 2025.

Lightning, hail, severe turbulence and severe icing associated with cumulonimbus clouds (Cb) present a significant safety hazard to air traffic and can impact the comfort and timeliness of a flight. The World Area Forecast System (WAFS) facilitates safe and efficient flight planning by providing global forecasts of key meteorological hazards. The next generation of WAFS will provide probabilistic forecasts of these hazards, including cumulonimbus clouds.

At the Met Office, these forecasts are currently made using three simple threshold tests applied to parameters from MOGREPS-G, a global NWP ensemble. These thresholds are used as a proxy for the occurrence of cumulonimbus clouds in the NWP data.

In this work, a series of deep learning models have been trained to predict the occurrence of cumulonimbus in global satellite observations using a wider set of parameters from the control member of MOGREPS-G. The purpose of the training is for the deep learning model to learn the representation of a cumulonimbus in the NWP data in a supervised manner. The model predictions are then applied to the whole ensemble to produce a probability forecast of cumulonimbus occurrence.

A range of loss functions were used during model training and verification to account for spatial information at a range of scales. Different loss functions were also used to enhance the reward for correct forecasts of the relatively rare cumulonimbus clouds.

Some of the trained models are shown to have greater skill than a baseline using the threshold test method. The model characteristics change depending on the choice of loss function used during training.

Further work is needed to explore how to make predictions at a range of lead times and how to use inputs from the whole ensemble.

How to cite: Creswick, A.: A deep learning approach for probabilistic forecasts of cumulonimbus clouds from NWP data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9783, https://doi.org/10.5194/egusphere-egu25-9783, 2025.

EGU25-9837 | Orals | AS1.1

Probabilistic Postprocessing of Hourly Precipitation Ensemble Forecasts Using UNet 

Marcos Esquivel González, Albano González, Juan Carlos Pérez, Juan Pedro Díaz, and Pierre Simon Tondreau

Title: Probabilistic Postprocessing of Hourly Precipitation Ensemble Forecasts Using UNet 

Authors: Marcos Esquivel-González, Albano González, Juan Carlos Pérez, Juan Pedro Díaz, Pierre Simon Tondreau

Affiliation of authors: Grupo de Observación de la Tierra y la Atmósfera (GOTA), Avenida Astrofísico Francisco Sánchez, s/n, La Laguna, 38200, Canary Islands, Spain

Abstract: Reliable precipitation forecasting is crucial in sectors like public safety, agriculture and water management. Numerical Weather Prediction (NWP) models, which form the backbone of modern forecasting, are prone to errors due to their limitations and the chaotic behavior of equations, requiring postprocessing to improve accuracy and quantify uncertainties. Thus, this study evaluates probabilistic postprocessing models tailored for the Canary Islands, with the aim of enhancing Weather Research and Forecasting (WRF) ensemble forecasting accuracy in hourly precipitation forecast. UNet-based models were explored using two approaches,  one incorporating  the full set of km-scale convection-permitting ensemble forecast simulations (25) and another applying dimensionality reduction via Principal Component Analysis (PCA) and feature selection methods. These models were compared to traditional benchmarks like the Censored Shifted Gamma Distribution (CSGD) with Ensemble Model Output Statistics (EMOS) and the Analog Ensemble method. In the analysis of the results, not only the reliability of the predictions for the set of available meteorological stations was considered, but also the generalization capacity of the UNet models to obtain precipitation predictions for the whole region.

In general, UNet models outperformed traditional approaches. The UNet with PCA excelled in probabilistic and deterministic metrics but struggled in regions without weather station data. Conversely, the UNet with feature selection, while slightly less accurate overall station locations, showed better generalization to unseen locations, maintaining consistent performance across the region and reducing computational demand. Additionally, the Integrated Gradients technique, an interpretability method that quantifies the contribution of each input feature to a model’s predictions by analyzing gradients, was employed to evaluate the impact of input variables on model performance. This analysis revealed that the integration of digital terrain elevation data significantly contributed to the UNet's outputs, underscoring the importance of topographic data in rainfall prediction.

How to cite: Esquivel González, M., González, A., Pérez, J. C., Díaz, J. P., and Tondreau, P. S.: Probabilistic Postprocessing of Hourly Precipitation Ensemble Forecasts Using UNet, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9837, https://doi.org/10.5194/egusphere-egu25-9837, 2025.

EGU25-10090 | Posters on site | AS1.1

Precipitation Downscaling Using Dynamical and Neural Network Approaches. 

Bijan Fallah and Masoud Rostami

High-resolution climate projections are crucial for assessing the future impacts of climate change. Statistical, dynamic, or hybrid climate data downscaling is often employed to create the datasets required for impact modelling. In this study, we utilize the COSMO-CLM (CCLM) version 6.0, a regional climate model, to investigate the advantages of dynamically downscaling a general circulation model (GCM) from CMIP6, with a focus on Central Asia (CA). The CCLM, running at a 0.22° horizontal resolution, is driven by the MPI-ESM1-2-HR GCM (at 1° spatial resolution) for the historical period 1985–2014 and projections for 2019–2100 under three shared socioeconomic pathways (SSPs): SSP1-2.6, SSP3-7.0, and SSP5-8.5 (Fallah et al., 2025). Using the CHIRPS gridded observation dataset for evaluation, we assess the performance of the CCLM driven by ERA-Interim reanalysis over the historical period.

The added value of CCLM, particularly over mountainous areas in CA, is evident, with a reduction in mean absolute error and bias of climatological precipitation by 5 mm/day for summer and 3 mm/day for annual values (Fallah et al., 2024). While no error reduction is achieved for winter, the frequency of extreme precipitation events improves in the CCLM simulations. Future projections indicate an increase in the intensity and frequency of extreme precipitation events in CA by the century’s end, particularly under the SSP3-7.0 and SSP5-8.5 scenarios. The number of days with more than 20 mm of precipitation increases by more than 90, and the annual 99th percentile of total precipitation increases by over 9 mm/day in mountainous areas.

A convolutional neural network (CNN) is also trained to map GCM simulations to their dynamically downscaled CCLM counterparts. The CNN successfully emulates the GCM-CCLM chain across large areas of CA but demonstrates reduced skill when applied to other GCM-CCLM chains. This downscaling approach and CNN architecture provide an alternative to traditional methods and could be a valuable tool for the scientific community involved in downscaling CMIP6 models (Harder et al., 2023).

In future work, we aim to extend this approach by training a neural network model to map the available GCM-RCM model chains for CORDEX-EU and applying the trained model to decadal prediction ICON simulations. This will enable the production of CORDEX-EU-like regional ICON simulations, bridging the gap between global and regional climate information on decadal timescales. By integrating decadal predictions into the framework, we aim to enhance the usability of regionalized climate data for short-term climate planning and decision-making.

References:

  • Fallah, B., Russo, E., Menz, C., Hoffmann, P., Didovets, I., and Hattermann, F. F.: Anthropogenic influence on extreme temperature and precipitation in Central Asia, Sci. Rep., 13, 6854, https://doi.org/10.1038/s41598-023-33921-6, 2023.
  • Fallah, B., Menz, C., Russo, E., Harder, P., Hoffmann, P., Didovets, I., and Hattermann, F. F.: Climate Model Downscaling in Central Asia: A Dynamical and a Neural Network Approach, Geosci. Model Dev. Discuss. [preprint], https://doi.org/10.5194/gmd-2023-227, accepted, 2025.
  • Harder, P., Hernandez-Garcia, A., Ramesh, V., Yang, Q., Sattegeri, P., Szwarcman, D., Watson, C., and Rolnick, D.: Hard-Constrained Deep Learning for Climate Downscaling, J. Mach. Learn. Res., 24, 1–40, 2023.

How to cite: Fallah, B. and Rostami, M.: Precipitation Downscaling Using Dynamical and Neural Network Approaches., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10090, https://doi.org/10.5194/egusphere-egu25-10090, 2025.

EGU25-10119 | ECS | Posters on site | AS1.1

Pavement Temperature Forecasts Based on Model Output Statistics: Experiments for Highways in Jiangsu, China 

Shoupeng Zhu, Yang Lyu, Hongbin Wang, Linyi Zhou, and Chengying Zhu

Forecasts on transportation meteorology, such as pavement temperature, are becoming increasingly important in the face of global warming and frequent disruptions from extreme weather and climate events. In this study, we propose a pavement temperature forecast model based on stepwise regression—model output statistics (SRMOS) at the short-term timescale, using highways in Jiangsu, China, as examples. Experiments demonstrate that the SRMOS model effectively calibrates against the benchmark of the linear regression model based on surface air temperature (LRT). The SRMOS model shows a reduction in mean absolute errors by 0.7–1.6 °C, with larger magnitudes observed for larger biases in the LRT forecasts. Both forecasts exhibit higher accuracy in predicting minimum nighttime temperatures compared to maximum daytime temperatures. Additionally, it overall shows increasing biases from the north to the south, and the SRMOS superiority is greater over the south with larger initial LRT biases. Predictor importance analysis indicates that temperature, moisture, and larger-scale background are basically the key predictors in the SRMOS model for pavement temperature forecasts, of which the air temperature is the most crucial factor in the model’s construction. Although larger-scale circulation backgrounds are generally characterized by relatively low importance, their significance increases with longer lead times. The presented results demonstrate the considerable skill of the SRMOS model in predicting pavement temperatures, highlighting its potential in disaster prevention for extreme transportation meteorology events.

How to cite: Zhu, S., Lyu, Y., Wang, H., Zhou, L., and Zhu, C.: Pavement Temperature Forecasts Based on Model Output Statistics: Experiments for Highways in Jiangsu, China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10119, https://doi.org/10.5194/egusphere-egu25-10119, 2025.

Raw forecasts, be they weather or hydrological, suffer from the inevitable errors stemming from either model structures or initial conditions estimation. With forecasting being a critical component in addressing challenges in flood control, reservoir and hydropower operation, and other fields related to the environment, energy and public safety, improving forecasting skill is increasingly necessary. Post-processing methods can help in this regard and can help improve forecast accuracy and reliability. Non-Homogeneous Gaussian Regression (NGR) and Bayesian Model Averaging (BMA) are the two most commonly used methods when it comes to post-processing probabilistic forecasts, and they have shown to be similarly efficient in many studies. For case studies where there are several distinct forecasts for one single observation, NGR risks losing information on uncertainty by aggregating the forecasts even though it accounts for heteroscedasticity. BMA, on the other hand, evaluates distinct model components and utilizes them accordingly, while assuming all the forecasts are alike in their under/overdispersion. This work introduces a mixed NGR-BMA approach for calibrating air temperature forecasts with lead-times of 1-10 days where the forecasts are first processed with NGR and then corrected once more by BMA according to a priori information on the skill of model components. This way, the upsides of each method is maintained through post-processing. The results generally show that the higher the lead-time, the more the proposed method outperforms either BMA or NGR taken individually. 

How to cite: Oghbaei, B. and Arsenault, R.: Using Non-Homogeneous Gaussian Regression to incorporate heteroscedasticity when post-processing air temperature forecasts by Bayesian Model Averaging, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10245, https://doi.org/10.5194/egusphere-egu25-10245, 2025.

EGU25-10701 | Orals | AS1.1

Leveraging Data-Driven Weather Forecasting for Improving Numerical Weather Prediction Skill Through Large-Scale Spectral Nudging 

Leo Separovic, Syed Husain, Jean-François Caron, Rabah Aider, Mark Buehner, Stéphane Chamberland, Charles Creese, Ervig Lapalme, Ron McTaggart-Cowan, Christopher Subich, Paul Vaillancourt, Jing Yang, and Ayrton Zadra

Operational weather forecasting has traditionally relied on physics-based numerical weather prediction (NWP) models, but the rise of AI-based weather emulators is reshaping this paradigm. However, most data-driven models for medium-range forecasting still face limitations, such as a narrow range of predicted variables and low effective spatiotemporal resolution. This presentation will compare the strengths and weaknesses of these two approaches, using Environment and Climate Change Canada’s Global Environmental Multiscale (GEM) model and Google DeepMind’s GraphCast model. It will demonstrate that GraphCast outperforms GEM in predicting large-scale features, particularly for longer lead times.

Building on these findings, we propose a new hybrid NWP-AI system, in which GEM’s large-scale state variables are spectrally nudged towards GraphCast’s inferences, while GEM continues to generate fine-scale details critical for weather extremes. Results show that this hybrid system improves GEM’s forecast accuracy, reducing RMSE for the 500-hPa geopotential height by 5-10% and extending predictability by 6-12 hours in the extratropics, peaking at day 7 of the forecast. It also yields significant improvements in tropical cyclone trajectory prediction without degrading intensity forecasts. Unlike state-of-the-art AI-based models, the hybrid system ensures meteorologists retain access to all forecast variables, including those critical for high-impact weather. Preparations are currently well underway for the operationalization of this hybrid system at the Canadian Meteorological Centre. 

How to cite: Separovic, L., Husain, S., Caron, J.-F., Aider, R., Buehner, M., Chamberland, S., Creese, C., Lapalme, E., McTaggart-Cowan, R., Subich, C., Vaillancourt, P., Yang, J., and Zadra, A.: Leveraging Data-Driven Weather Forecasting for Improving Numerical Weather Prediction Skill Through Large-Scale Spectral Nudging, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10701, https://doi.org/10.5194/egusphere-egu25-10701, 2025.

EGU25-11378 | Orals | AS1.1

The Role of Water Vapour in Shaping Mediterranean Summer Climate: Findings from MESSA-DIN 2021 measurement campaing in southern Italy 

Fabio Madonna, Ilaria Gandolfi, Marco Rosoldi, Faezeh Karimian Saracks, Yassmina Hesham Essa, and Giada Salicone

Water vapour fluxes, originating mainly from the Atlantic, North Africa, and the Mediterranean region, play a critical role in shaping the climate dynamics of the Mediterranean Basin, especially during the summer months. These fluxes significantly influence relative humidity levels in the troposphere, affecting both local and regional weather patterns, such as intense rainfall events and prolonged droughts, while also contributing to the amplification of heatwaves through enhanced surface radiation trapping. This study uses observational data collected during the Mediterranean Experiment for Sea Salt and Dust Ice Nuclei (MESSA-DIN) from July to September 2021 in Soverato, southern Italy, to characterise the synoptic conditions of the severe summer of 2021.

A combination of ground-based remote sensing instruments revealed intense and persistent water vapour transport in the mid-troposphere. ERA5 data were used to identify the moisture dynamics over the Mediterranean Basin. The comparison between ERA5 reanalysis data and ground-based measurements further highlighted discrepancies in the representation of water vapour, particularly a dry bias in relative humidity in the range between 500 hPa and 300 hPa. While ERA5 provided a coherent and detailed representation of synoptic patterns and showed general agreement in the time evolution of the atmospheric vertical structure with observations, it exhibited a dry bias in relative humidity (RH) values compared to a ground-based microwave profiler (MWP). However, the magnitude of the bias also depends on the bias affecting the MWP retrieval, typically within 10-15% RH in the mid-troposphere. ERA5 also overestimates the presence of both cold and warm clouds, while ground instruments detected much less frequent cloud cover. This emphasizes the need for improving reanalysis performance in complex coastal and orographic settings. The bias in ERA5 was further assessed using GRUAN data from the Potenza station and regular upper-air data from Mediterranean stations.

The study underscores the importance of ground-based measurements, such as those from microwave radiometers, in improving weather forecasts for extreme events. Despite their lower vertical resolution, these instruments—both on their own and when combined with higher-resolution measurement techniques such as Raman lidars and upper-air soundings—provide continuous, real-time measurements of atmospheric water vapour. These measurements are essential for enhancing our understanding of water vapour fluxes and their impact on cloud formation, as well as for improving the accuracy of high-resolution forecasting models, especially in the representation of extreme weather events in the Mediterranean and Central Europe.

How to cite: Madonna, F., Gandolfi, I., Rosoldi, M., Karimian Saracks, F., Hesham Essa, Y., and Salicone, G.: The Role of Water Vapour in Shaping Mediterranean Summer Climate: Findings from MESSA-DIN 2021 measurement campaing in southern Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11378, https://doi.org/10.5194/egusphere-egu25-11378, 2025.

EGU25-12077 | ECS | Orals | AS1.1 | Highlight

The AIFS: ECMWF’s data-driven weather forecasting system 

Sara Hahner and the AIFS-Team

Machine learning-based models are rapidly transforming medium-range weather forecasting. The European Centre for Medium-Range Weather Forecasts (ECMWF) has developed the Artificial Intelligence Forecasting System (AIFS), a state-of-the-art data-driven model combining a graph neural network encoder-decoder with a sliding window transformer processor. Trained on ECMWF's ERA5 re-analysis and operational numerical weather prediction analyses, AIFS demonstrates exceptional deterministic forecast skill across upper-air variables, surface weather parameters, and tropical cyclone tracks.

Building on this foundation, ECMWF has introduced AIFS-CRPS, a probabilistic extension of AIFS designed for ensemble forecasting. AIFS-CRPS is obtained by training a stochastic model with the Continuous Ranked Probability Score (CRPS) as its loss function. It addresses uncertainties and generates highly skilful probabilistic forecasts. For medium-range timescales, AIFS-CRPS matches or outperforms ECMWF’s physics-based Integrated Forecasting System ensemble across key variables and lead times.

This presentation will highlight recent advancements in deterministic and probabilistic forecasting with AIFS, showcasing its operational readiness and its potential to redefine medium-range forecasting at ECMWF.

How to cite: Hahner, S. and the AIFS-Team: The AIFS: ECMWF’s data-driven weather forecasting system, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12077, https://doi.org/10.5194/egusphere-egu25-12077, 2025.

EGU25-13191 | ECS | Orals | AS1.1

Using VIL density for identification of storm nuclei, tracking and nowcasting in the Barcelona Metropolitan Area 

Laura Esbri, Tomeu Rigo, Montserrat Llasat-Botija, and María Carmen Llasat

Urban resilience to extreme weather events is increasingly threatened by the intensification of short-duration rainfall, often leading to urban flooding. This study focuses on improving the prediction of heavy rainfall in the Metropolitan Area of Barcelona, located on the Catalan Mediterranean coast in the northeast of the Iberian Peninsula, using high-resolution radar products and rain gauge data. Despite the decrease in average of annual rainfall in the AMB over recent decades, the intensity rates of some storm events are among the highest of the existing series, with occasional convective events causing urban flooding and severe disruptions for the urban region. The latest climate change reports (IPCC 2022) point towards an increase in frequency and intensity of heavy rainfall events in the region.

An extensive dataset of rainfall days spanning from 2014 to 2022 is analysed, including volumetric radar products (VIL, Echo Top), surface rainfall measurements, and incident reports. A bottom-up approach is used to identify 45 intense convective days with significant impacts in the study region. A radar-based nowcasting approach is introduced, utilizing a two-dimensional radar product with three-dimensional atmospheric information to enhance early warnings in the urban region, with high spatial resolution. This approach focuses on the convective parts of storms through Vertical Integrated Liquid (VIL) density-based tracking and nowcasting with six-minute temporal updates to characterize storm centroids and their evolution. The density of VIL (DVIL), derived from radar composites, provides vertical storm structure information in a two-dimensional format, enabling faster data processing without losing volumetric capabilities.

The findings reveal spatial coherence between maximum DVIL intensities and maximum rainfall locations, with all events exceeding the 2.5 g/m³ DVIL threshold coinciding with high-intensity rainfall. Centroid trajectories show seasonal patterns, with some summer events originating from scattered sources and moving more slowly, while some autumn ones align along the coast and propagating inland. The time lag between initial DVIL detection and peak precipitation for the analysed days ranges from 30 minutes to over two hours, offering critical lead times for early warnings.

This study demonstrates the strengths and limitations of DVIL as a predictor of heavy rainfall in urban areas. The RaNDeVIL module shows promise for operational nowcasting, with necessary improvements to address complex interactions of the storm dynamics and more complex modelling to nowcast longer timescales. These advancements aim to enhance resilience to intense precipitation in the Metropolitan Area of Barcelona under changing climatic conditions.

 

This project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement 101037193.

How to cite: Esbri, L., Rigo, T., Llasat-Botija, M., and Llasat, M. C.: Using VIL density for identification of storm nuclei, tracking and nowcasting in the Barcelona Metropolitan Area, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13191, https://doi.org/10.5194/egusphere-egu25-13191, 2025.

EGU25-13477 | Posters on site | AS1.1

Impact of climate change on ERA5 cloud cover and convective parameters in Central Europe (1983-2022) 

Virág Soós and Breuer Hajnalka

In discussions about climate change, the focus is usually on rising temperatures. However, it is important to understand the significant impact of climate change on the entire weather system. The cloud feedback mechanism is one of the most complex factors in the climate system. This is because clouds can have a heating and cooling effect at the same time, and this balance has a significant influence on the global radiation balance. To understand how all the different factors work together to create a complex system, we need to look closely at how these factors have changed over time.

The aim of this research is to examine changes in cloud cover and convective parameters, as well as the background, causes and effects of these changes in Central Europe between 1983 and 2022. The research uses data from the ERA5 reanalysis database. Aside from the analysis of environmental conditions, an objective cyclone identifying method is used to determine regions under low- or high-pressure weather system influence.  

The statistical analysis shows that in general, the decrease in ERA5 low-level cloud cover is associated with an increase in cloud base. Medium- and high-level cloud cover, however, is influenced by changes in large-scale circulation systems.

Low-level cloud cover decrease in the northern regions of the study area is likely due to increasing temperatures and decreasing boundary layer humidity. Though temperatures in the Mediterranean region also have risen, the increase in the frequency of negative NAO situations, and an increase in Mediterranean cyclone and low-pressure system activity - the latter of which is likely induced by the higher evaporation of the Mediterranean Sea - resulted in the increase in cloud cover over the central Mediterranean region. We have also observed an increase in the CAPE (convective area pressure energy) in the Mediterranean during the summer months, which leads to an increase in the frequency of heavy thunderstorms and extreme precipitation events in this area, contributing to the intensification of weather extremes in the region. Changes over the study area are not linear but show a region dependent 10-20 years periodical pattern which is also investigated.

How to cite: Soós, V. and Hajnalka, B.: Impact of climate change on ERA5 cloud cover and convective parameters in Central Europe (1983-2022), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13477, https://doi.org/10.5194/egusphere-egu25-13477, 2025.

Based on hourly precipitation data, the warm-sector rainfall events in Beijing-Tianjin-Hebei region are selected and classified using objective methods. There are 33 warm-sector rainfall events in this region from 2010 to 2023. They mainly occur during June and August with the most in July. The average lifetime of these warm-sector rainfall events is 5.44 h. The warm-sector rainfall events are mainly concentrated in the center of the Beijing-Tianjin-Hebei region, and the frequency of occurrence in the east is higher than that in the west. The frequency of occurrence in Beijing is much higher than that in other regions, and it is mainly concentrated in the terrain bell mouth of northeast Beijing. According to the circulation situation that generates warm-sector rainfall, three types of precipitation are obtained: low-vortex type, shear-line type and southerly-wind type. The occurrence months, starting times and locations of warm-sector rainfall events in different types are slightly different. Based on the analysis of the synthetic circulation situation, the dynamic, water vapor and low-level vertical motion conditions of the low-vortex type is most favorable for warm-sector rainfall. The vertical upward movement of shear line warm-sector rainfall events is strong in Beijing; The dynamic condition of southerly-wind type is the weakest, but the water vapor condition is more favorable and the occurrence is related to the topographic distribution of  Beijing-Tianjin-Hebei.

How to cite: Liu, R.: Selection and Classification of Warm-Sector Rainfall Events in Beijing-Tianjin-Hebei, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14147, https://doi.org/10.5194/egusphere-egu25-14147, 2025.

Precipitation nowcasting, which entails high-resolution forecasting of precipitation events within 1–2 hours, is significant to daily life and professional activities. Nevertheless, accurate short-term precipitation forecasting remains a considerable challenge at present. Traditional numerical weather prediction, which relies on intricate physical equations to simulate the Earth's atmospheric state, necessitates substantial computational resources and frequently yields lower accuracy for small-scale forecasts, thereby failing to meet the demands of precipitation prediction in complex regions. Most deep learning methodologies concentrate exclusively on the spatiotemporal prediction of a singular precipitation variable, thereby neglecting the dynamic spatiotemporal relationships between precipitation and other meteorological data within the meteorological system. Moreover, due to the rapid pace of climate change, long-term time series data is often inadequate for accurately addressing precipitation forecasting for extreme weather events, since past meteorological time series data may not accurately reflect the current atmospheric conditions. There is an urgent need to rely on short-term time series for prediction tasks. However, most current methods that rely on short-term time series for prediction perform poorly in forecasting moderate to heavy precipitation events. Inspired by spatiotemporal information transformation schemes, we introduce a spatiotemporal information(STI) transformation equation from chaotic dynamics into the field of computer vision and develop a neural network model framework based on spatiotemporal information transformation. This framework maps high-dimensional spatial information to the temporal information of future precipitation information, thereby facilitating the integration of dynamic spatiotemporal relationships between various meteorological data and precipitation, and enabling the mutual transformation of spatiotemporal information for enhanced forecasting accuracy. Furthermore, we propose an adaptive gradient loss function designed to improve the model's sensitivity to learning moderate-intensity precipitation. This research utilizes the US SEVIR dataset for training and testing, which encompasses data such as satellite visible light, infrared temperature, humidity, and cloud precipitation while employing multiple meteorological data for precipitation forecasting over the subsequent hour. We selected the Structural Similarity Index, Peak Signal-to-Noise Ratio, False Alarm Rate, Critical Success Index, and Heidke Skill Score as both quantitative and qualitative evaluation metrics. Experimental results demonstrate that the STI framework reduces the model's error in moderate to heavy precipitation events, making the model more sensitive to severe rainfall events. Furthermore, when the STI framework is integrated into other deep learning models and retrained, it further enhances their precipitation prediction accuracy. This finding indicates that the STI framework effectively captures the dynamic spatiotemporal relationships between various meteorological and precipitation data.

How to cite: Hu, J., Liu, D., Huang, X., and Wu, X.:  Spatiotemporal Information Transformation for Precipitation Nowcasting Using Multi-Meteorological Factors, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14517, https://doi.org/10.5194/egusphere-egu25-14517, 2025.

Moist convection in the Maritime Continent (MC) is typically driven by synoptic disturbances: Northerly Cold Surge (NCS), Borneo Vortex, and Madden-Julian Oscillation (MJO). One or more of these tropical disturbances can control the convective behaviour in the MC, resulting in changes in the diurnally forced convection, cloud populations and diurnal precipitation. This investigation analyses a record extreme rainfall event on Java Island around New Year's Eve 2020, the highest amount of rainfall recorded in the capital city of Indonesia, Jakarta. We use reanalysis data from ECMWF Reanalysis v5 (ERA5) to identify and analyse the southward propagation of the NCS. Satellite measurements from the Himawari-8 Advanced Himawari Imager and satellite-derived cloud physical properties reveal the cloud signatures of the NCS. High-resolution Weather Research & Forecasting Model (WRF) simulations were performed to understand the mesoscale dynamic process of the NCS's interaction with the enhanced precipitation at the diurnal scale.

Our results suggest that this extreme event resulted from the interaction of an NCS event and the diurnally forced convection. A persistent northwesterly wind near the surface over the Java Sea induced an intense low-level wind convergence from the meridional moisture transport associated with the NCS and the equatorial trough over Java. This promoted the necessary unstable conditions for organised convection during the afternoon-evening. The cloud populations and diurnal cycle of heavy rainfall in western Java were affected by the frontal region of the NCS with the offshore propagating land breeze from Java and Sumatra, as well as the intense convergence of moisture air in the internal seas of the MC. Our analysis also suggests that the presence of this strong cross-equatorial flow in the MC induced moisture transport from the southern part of Sumatra to the western region of Java. The findings outlined here could be utilised to enhance our understanding of severe weather in the MC.

How to cite: Lopez-Bravo, C.: A high-resolution modelling and observational analysis of an extreme rainfall event driven by the Northerly Cold Surge and intraseasonal tropical variability in Jakarta: January 2020, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14567, https://doi.org/10.5194/egusphere-egu25-14567, 2025.

EGU25-15060 | Orals | AS1.1

Fair Box ordinate transform for multivariate Gaussian forecasts 

Sándor Baran and Martin Leutbecher

In evaluating multivariate probabilistic forecasts predicting vector quantities such as a weather variable at multiple locations or a wind vector, an important step is the assessment of their calibration and reliability. Here, we focus on the Gaussian Box ordinate transform (BOT), which is appropriate if the forecasts and observations are multivariate normal. The BOT is based on the Mahalanobis distance of the observation vector and the estimated Gaussian mean and asymptotically standard uniform if the forecasts and the observation are drawn from the same multivariate Gaussian law. However, for small ensemble sizes combined with high dimensionality, deviation from uniformity is substantial even for reliable forecasts, resulting in hump-shaped or triangular BOT histograms. To circumvent this problem, we derive an ensemble size and dimension-dependent fair version of the Gaussian BOT, where the uniformity holds for any combination of these parameters. With the help of a simulation study, first, we assess the behaviour of the fair BOT for various dimensions, ensemble sizes, and types of calibration misspecification. Then, using ensemble forecasts of vectors consisting of multiple combinations of upper-air weather variables, we demonstrate the usefulness of the fair BOT when multivariate normality is only an approximation.

*Research was supported by the Hungarian National Research, Development and Innovation Office under Grant No. K142849.

How to cite: Baran, S. and Leutbecher, M.: Fair Box ordinate transform for multivariate Gaussian forecasts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15060, https://doi.org/10.5194/egusphere-egu25-15060, 2025.

EGU25-15639 | Posters on site | AS1.1

Ensemble Convective Rainfall Nowcasting by integrating Numerical Weather Prediction models and Neural Networks: the ICREN project 

Giovanna Venuti, Xiangyang Song, Stefano Federico, Giorgio Guariso, Matteo Sangiorgio, Claudia Pasquero, Seyed Hossein Hassantabar Bozroudi, Ali Badr Eldin Ali Mohamed, Ruken Dilara Zaf, Lorenzo Luini, Roberto Nebuloni, and Eugenio Realini

Convective events pose a significant threat to society due to the associated heavy rainfall, large hail, strong winds, and lightning. Location and timing determination of convective precipitation is still a challenge for modern meteorology. Despite the good skills of current weather forecasting tools in the prediction of the large-scale environment facilitating the onset of convective phenomena, the multitude of spatial scales involved in such events makes their characterization, observation, and forecast a difficult task. The problem is further complicated by their rapid temporal development, which lasts from minutes to a few hours depending on the specific case.

Recent research indicates that the predictability of these events can be strongly improved accounting for local meteorological observations. 

The goal of the ICREN (Intense Convective Rainfall Events Nowcasting) project is to enhance the nowcasting of convective events by:

  • exploiting the information made available by local standard and non-conventional observations of meteorological variables
  • integrating physically based Numerical Weather Prediction (NWP) models with data-driven black box Neural Networks (NNs). 

The NWP model is used to support the NN by means of pseudo-observations (forecasted variables); while the fast computational speed of the NN enables advancing predictions in time and generating ensemble forecasts of convective phenomena.

The project is carried out in the Seveso River basin (almost 300 km2) in Northern Italy. In this region, convective events trigger floods and flash floods heavily impacting the large urban area of Milan.

Within the project, the Weather Research and Forecasting (WRF) NWP model is employed. By using three nested grids, the model achieves a 2 kkm x 2 km spatial resolution over the test area. To optimize the prediction of meteorological variables required by the NN, the model assimilates lightning observations and GNSS-derived Zenith Tropospheric Delays (ZTDs), both of which enhance the representation of local atmospheric humidity.

Several NN models have been trained on standard meteorological data, GNSS ZTDs, and radar-derived parameters—including the position, velocity, and attenuation of convective cells—to identify the architecture best suited for predicting 10-minute accumulated rainfall from 10 minutes up to 1 hour following the detection of a convective event in the test area.

The best-performing models are used to generate ensemble predictions of rainfall events by suitably perturbing the input variables.

Results from the WRF model, the NN predictions and the ensemble forecasts will be presented along with initial integration outcomes for selected convective events occurring in the test area in 2019.

 

This work is supported by the ICREN-PRIN project (MUR- CUP: D53D23004770006). 



How to cite: Venuti, G., Song, X., Federico, S., Guariso, G., Sangiorgio, M., Pasquero, C., Hassantabar Bozroudi, S. H., Mohamed, A. B. E. A., Zaf, R. D., Luini, L., Nebuloni, R., and Realini, E.: Ensemble Convective Rainfall Nowcasting by integrating Numerical Weather Prediction models and Neural Networks: the ICREN project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15639, https://doi.org/10.5194/egusphere-egu25-15639, 2025.

Mesoscale vortices in the boundary layer are characterized by short lifespans, small spatial scales, and difficulty in prediction, leading to their frequent oversight in operational forecasting. This oversight often results in lower accuracy for precipitation forecasting associated with these vortices. From April 2 to April 3 2023, a squall line event triggered by vortices extending from the lower troposphere to the boundary layer occurred across eastern Hubei to western Anhui. This event developed ahead of a shallow mid-tropospheric trough, while the lower levels were influenced by southwest flow. High-resolution numerical simulations successfully reproduced the evolution of the vortex and the organizational development of the squall line. Dynamic diagnosis revealed that the nocturnal boundary layer vortex (925 hPa) was initiated by the intensification of the nocturnal jet and the blocking effect of terrain. Subsequently, through vertical advection of horizontal vorticity from boundary layer to lower level, the vortex at the lower troposphere (850 hPa) developed and intensified. Later, under the combined influence of horizontal divergence and horizontal advection, the vortex rapidly strengthened, creating favorable convergence conditions for the squall line's development due to the northerly flow west of the vortex and the southwest flow south of it.

How to cite: Zhang, Y., Xi, X., and Sun, J.: The formation and evolution mechanism of the boundary layer vortex east of thesecond-step terrain along the middle reaches of the Yangtze River, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15786, https://doi.org/10.5194/egusphere-egu25-15786, 2025.

EGU25-15861 | ECS | Orals | AS1.1

Improving seasonal forecasts for early warning systems in Germany 

Yanet Díaz Esteban, Qing Lin, Fatemeh Heidari, Edgar Fabián Espitia Sarmiento, and Elena Xoplaki

Climate forecasts at seasonal timescales are critical for various sectors, and play a key role in decision-making processes, helping to mitigate risks associated with climate variability and extreme events. However, model outputs are typically insufficient for many practical applications due to coarse resolution and systematic biases, requiring the employment of post-processing techniques to enhance their usability and target stakeholders’ interest such as early warning systems. Post-processing techniques such as downscaling and bias correction can translate model outputs into higher-resolution, bias-corrected forecasts that are more relevant and best appropriate for local applications. We present a physics-informed CNN-based framework for downscaling and bias correction of ECMWF SEAS5.1 seasonal temperature and precipitation forecasts over Europe from 1° to ~1.2km, which represents a downscaling factor of ~60. The approach considers several climate drivers of atmospheric surface variables from SEAS5.1 as input and takes European Meteorological Observations at 1.2 km as ground truth data. We use an analog-based approach to account for the mismatch between long-range model outputs and observations due to model drifting, which is a problem for supervised neural networks algorithms running on climate datasets. Finally, we present a detailed evaluation of the performance for the period 2017-2022, by comparing our results to the raw output. In most cases, the post-processed forecasts outperform the raw predictions in terms of bias reduction, spatial representation and capturing the extremes. This work has potential implications for reducing uncertainties, improving spatial representation, and addressing systematic biases present in raw ECMWF seasonal products.

How to cite: Díaz Esteban, Y., Lin, Q., Heidari, F., Espitia Sarmiento, E. F., and Xoplaki, E.: Improving seasonal forecasts for early warning systems in Germany, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15861, https://doi.org/10.5194/egusphere-egu25-15861, 2025.

EGU25-16130 | Posters on site | AS1.1

Enhancing Radar-Based Precipitation Nowcasting Model with AI-Predicted Precipitation Intensity Change Rates 

Kwang-Ho Kim, Kyeongyeon Ko, and Kyung-Yeub Nam

The importance of precipitation nowcasting is gradually expanding due to the increasing frequency and intensity of localized rainfall caused by climate change. The growth and decay processes of precipitation are critical factors influencing the accuracy of precipitation nowcasting, necessitating advanced modeling approaches. This study proposes a novel methodology that integrates artificial intelligence (AI) with high-resolution radar data to predict the growth and decay processes of precipitation, incorporating these predictions into a radar-based nowcasting model. In this study, AI was applied to predict radar-based precipitation intensity change rates up to two hours ahead, and these predictions were integrated into a precipitation nowcasting model. The AI effectively learned the spatiotemporal patterns of nonlinear precipitation evolution using the RainNet architecture. The AI was trained on three years (2021 – 2023) of radar-derived precipitation intensity change rates, with one year (2020) used for validation to evaluate its performance. The nowcasting model was developed using cross-correlation techniques to calculate motion vectors of the precipitation system at different spatial scales, and a semi-Lagrangian backward extrapolation method was employed for precipitation prediction. Integrating AI-predicted precipitation intensity change rates into the nowcasting model resulted in significant improvements in prediction performance. The results showed a 10% improvement in precipitation prediction accuracy compared to the baseline nowcasting model that did not incorporate AI-based precipitation intensity change rate predictions. The model effectively captured rapid changes in precipitation intensity, demonstrating the utility of AI-based predictions for short-term nowcasting. This study highlights the potential of combining traditional nowcasting models with AI techniques, presenting a promising approach for enhancing precipitation prediction accuracy.

This research was supported by the "Development of radar based severe weather nowcasting technology (KMA2021-03122)" of "Development of integrated application technology for Korea weather radar" project funded by the Weather Radar Center, Korea Meteorological Administration.

How to cite: Kim, K.-H., Ko, K., and Nam, K.-Y.: Enhancing Radar-Based Precipitation Nowcasting Model with AI-Predicted Precipitation Intensity Change Rates, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16130, https://doi.org/10.5194/egusphere-egu25-16130, 2025.

EGU25-16651 | Orals | AS1.1

RUSH: A Novel Fully AI-driven Framework for Seamless Integration of Observations and Global AI Forecasts in Short-term Weather Prediction 

Gabriele Franch, Elena Tomasi, Simon de Kock, Matteo Angelinelli, and Marco Cristoforetti

Short-term weather forecasting, especially for extreme events, remains challenging due to the need to effectively combine recent observations with numerical weather predictions. To tackle this challenge, we present RUSH (Rapid Update Short-term High-resolution forecast), an innovative framework designed to provide high-resolution (1 km) precipitation forecasts on a national scale with lead times up to 24 hours. RUSH follows the recent attempts to create fully AI-driven kilometer-scale forecasting systems that completely replace traditional numerical modeling with a combination of machine learning and observational data. Our system employs a Latent Diffusion Model architecture to seamlessly blend information from multiple data sources, including radar composites, satellite observations (SEVIRI bands), and ECMWF's AI-based global forecasting system (AIFS). 

The model is conceptually designed to transition from observation-driven predictions in the first few hours to a sophisticated spatial and temporal downscaling of AIFS forecasts at longer lead times. This approach aims to leverage the strengths of both data sources: the high spatial and temporal resolution of observational data for immediate forecasts, and the physically consistent evolution provided by AIFS for longer horizons. By utilizing an end-to-end AI architecture from global to local scale, RUSH not only addresses the computational constraints typically associated with traditional numerical weather predictions but also explores the potential for a new generation of fully data-driven weather forecasting systems. 

Our framework processes multi-source input data at different spatial and temporal scales, including radar-derived 30-minute precipitation accumulations, key SEVIRI channels, and selected AIFS forecast fields at 25km resolution. The model's sequence-to-sequence architecture allows for flexible spatial domain handling and probabilistic precipitation forecasting through multiple realizations. 

We will present preliminary results from two experimental implementations over different European domains (Italy and Belgium), demonstrating the model's capability to generate rapid-update forecasts and discussing its potential for operational implementation in weather services. The evaluation will focus on precipitation prediction skills across different intensity thresholds and temporal scales, with particular attention to extreme event forecasting. A preliminary comparison with operational limited area models (COSMO-2I and ALARO-AROME) over selected case studies will assess the competitiveness of this fully AI-driven approach against high-resolution numerical weather prediction systems. 

How to cite: Franch, G., Tomasi, E., de Kock, S., Angelinelli, M., and Cristoforetti, M.: RUSH: A Novel Fully AI-driven Framework for Seamless Integration of Observations and Global AI Forecasts in Short-term Weather Prediction, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16651, https://doi.org/10.5194/egusphere-egu25-16651, 2025.

EGU25-16934 | ECS | Posters on site | AS1.1

Clustering-based spatial interpolation of parametric post-processing models 

Mária Nagy-Lakatos and Sándor Baran

Parametric approaches to post-processing methods are widely used today, as they provide full predictive distributions for the weather variable of interest. These methods rely on training data consisting of historical forecast-observation pairs to estimate their parameters. Consequently, post- processed forecasts are generally restricted to locations with accessible training data. To overcome this limitation, we introduce a general clustering-based interpolation technique that extends calibrated predictive distributions from observation stations to any location within the ensemble domain where ensemble forecasts are available. Using the ensemble model output statistics (EMOS) post-processing technique, we conduct a case study based on 10-m wind speed ensemble forecasts from the European Centre for Medium-Range Weather Forecasts.  The results illustrate the effectiveness of the proposed method, demonstrating its advantages over both regionally estimated and interpolated EMOS models as well as raw ensemble forecasts.

Reference:  Baran, S. and Lakatos, M. (2024) Clustering-based spatial interpolation of parametric post-processing models. Wea. Forecasting  9, 1591-1604.

Research was supported by the Hungarian National Research, Development and Innovation Office under Grant No. K142849.

How to cite: Nagy-Lakatos, M. and Baran, S.: Clustering-based spatial interpolation of parametric post-processing models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16934, https://doi.org/10.5194/egusphere-egu25-16934, 2025.

EGU25-17194 | ECS | Orals | AS1.1

Exploring spatiotemporal vector autoregressive models for radar nowcasting 

Viv Atureta, Stefan Siegert, and Peter Challenor

Radar nowcasting methodologies have evolved from traditional optical flow and extrapolation techniques to advanced deep learning algorithms. However, accurately modeling growth and decay processes remains a significant challenge. This study explores spatio-temporal statistical models inspired by physics-based stochastic partial differential equations (SPDEs). Specifically, the solution to the advection-diffusion PDE is framed as a vector autoregressive process with coloured noise, characterized by non-uniform spectral properties.

We investigate the stochastic component using Gaussian Processes (GPs) and Gauss Markov Random Fields (GMRFs), evaluating covariance structures such as exponential, squared exponential, and dynamically weighted covariance and precision matrices. Nowcasts employing state-dependent GPs and GMRFs are assessed over lead times ranging from 15 minutes to 2 hours. The approach is tested on simulated data and UK precipitation events from the Met Office Nimrod system, focusing on a 200 km × 200 km region. Training data spans January 2014 to December 2020, with observational dimensions on the order of 10^4. To enable computationally efficient Bayesian inference, we utilize sparse matrix methods and Laplace approximations.

How to cite: Atureta, V., Siegert, S., and Challenor, P.: Exploring spatiotemporal vector autoregressive models for radar nowcasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17194, https://doi.org/10.5194/egusphere-egu25-17194, 2025.

EGU25-17279 | ECS | Posters on site | AS1.1

Nowcasting precipitation events from mesoscale convective systems for Dakar, Senegal  

Mai-Britt Berghöfer, Diana L. Monroy, and Jan O. Härter

Senegal, located in the West Sahel region, frequently experiences flooding driven by mesoscale convective systems (MCSs), which contribute 90% of the region’s rainfall. Current early warning systems for hydrological extremes struggle with timely and accurate predictions, necessitating advancements in precipitation nowcasting. Nowcasting describes short-term weather forecasts with a lead time of typically less than two hours. In this region traditional numerical weather models have limited accuracy in predicting short-term events, and nowcasting models therefore outperform numerical weather prediction in this time frame. Precipitation nowcasts can be helpful in supporting and informing decision makers on time to adapt to the risk and protect society from hydrological extremes.

A major challenge in developing warning systems for this region is the lack of radar data coverage, which is typically used in nowcasting models, compounded by a sparse ground-based observational network. Increasing the data availability and understanding the properties of MCSs could enhance the predictability of regional weather conditions, which is a primary objective of the High-resolution weather observations East of Dakar (DakE)-project. During the project, 14 automated weather stations have already been installed east of Dakar.

The objective of this study, which is part of the DakE-project, is to integrate the in-situ station data with satellite data to develop a precipitation nowcasting model that is optimally adapted to local conditions considering different spatial and temporal scales. An optical flow routine, based on statistical extrapolation of the current state of the atmosphere, is used for this purpose. To incorporate a stochastic term, which represents the unpredictable component, the STEPS (short-term ensemble prediction system) approach is applied. The skill of the forecast depends, among other things, on the geographical location, the spatial and temporal scales and the meteorological conditions, since developments that do not fulfil the steady-state assumption, such as the initiation, growth and termination of convective systems, are not resolved. The next step is to investigate whether these shortcomings can be compensated by implementing machine learning approaches.

 

References:

 

Anderson, Seonaid R., et al. "Nowcasting convective activity for the Sahel: A simple probabilistic approach using real‐time and historical satellite data on cloud‐top temperature." Quarterly Journal of the Royal Meteorological Society150.759 (2024): 597-617.

Mathon, V., Laurent, H., & Lebel, T. (2002). Mesoscale convective system rainfall in the Sahel. Journal of Applied Meteorology and Climatology41(11), 1081-1092.

Pulkkinen, S., Nerini, D., Pérez Hortal, A. A., Velasco-Forero, C., Seed, A., Germann, U., & Foresti, L. (2019). Pysteps: An open-source Python library for probabilistic precipitation nowcasting (v1. 0). Geoscientific Model Development12(10), 4185-4219.

Taylor, Christopher M., et al. "Nowcasting tracks of severe convective storms in West Africa from observations of land surface state." Environmental Research Letters 17.3 (2022): 034016.

 

 

Keywords: Nowcasting, Senegal, Mesoscale Convective System, Precipitation

How to cite: Berghöfer, M.-B., Monroy, D. L., and Härter, J. O.: Nowcasting precipitation events from mesoscale convective systems for Dakar, Senegal , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17279, https://doi.org/10.5194/egusphere-egu25-17279, 2025.

EGU25-17282 | ECS | Orals | AS1.1

Hybrid Post-Processing for Solar Power: Bridging Nowcasting to Short-Range   

Petrina Papazek, Pascal Gfäller, and Irene Schicker

Accurate forecasting of solar power generation is crucial for grid operators, as location-dependent photovoltaic (PV) installations exhibit diverse production patterns. The need for high temporal and spatial resolution, combined with the inherent variability of PV outputs, presents significant challenges for forecasting and post-processing across different time horizons. This study addresses these challenges in post-processing optimal point forecasts for PV sites across multiple forecasting ranges, with the aim of providing seamless output for end-users in the energy sector. Specifically, we focus on two-day-ahead PV site forecasts, with an emphasis on a highly resolved nowcasting range (from minutes to hours ahead) and a smooth transition to short-range forecasts. Advanced machine learning techniques, gridded meteorological models, and a variety of location-specific data sources are employed to enhance our post-processing approach for optimal site forecasts.

Focusing on an Austrian case study, we develop a post-processing framework based on machine learning approaches for time-series forecasting, with particular emphasis on Long Short-Term Memory (LSTM) models compared to more classical methods such as Random Forest (RF) and Multiple Linear Regression (MLR). Our primary objective is to smoothly post-process and identify transitions among a set of range-specific, mostly gridded background models spanning various spatial and temporal resolutions. The post-processed models used as input primarily represent irradiance and related parameters. Our work integrates IrradPhyD-Net, a high-resolution AI-based nowcasting model, with AROME, a limited-area Numerical Weather Prediction (NWP) model for the alpine region, providing valuable physical information extending into the short- and medium-range. To exploit the location-specific characteristics of the site, we incorporate additional time-series models that capture the climatology and trends of PV, irradiance, and strongly correlated parameters identified during pre-processing. Given the substantial and growing input data needs of AI and machine learning, we build on our previous contributions by integrating semi-synthetic data to address challenges posed by limited or inconsistent historical PV data, thereby improving model stability. In this context, additional data sources, such as satellite-based CAMS radiation time-series and ERA-5 reanalysis, are essential.

By leveraging skillful input models, supported by synthetic data, our post-processing framework demonstrates strong forecast skill across the studied ranges. Thus, sourcing and transforming data from multiple inputs proves to be an effective way to achieve seamless, high-skill forecasts while maintaining high temporal resolution for nowcasting.

How to cite: Papazek, P., Gfäller, P., and Schicker, I.: Hybrid Post-Processing for Solar Power: Bridging Nowcasting to Short-Range  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17282, https://doi.org/10.5194/egusphere-egu25-17282, 2025.

Gridscale forecasts of surface weather delivered by operational global NWP suffer from biases which depend strongly on the weather situation and on geographical factors. Such biases also plague re-analyses, such as ECMWF’s ERA5, as operational models are the engines of those re-analyses. This presentation will itemise a number of different gridscale biases identified through a conditional verification exercise in which millions of station measurements were compared with short range Control run forecasts of the ECMWF operational ensemble. We will postulate what physical reasons might underpin these biases. There is for example a strong dependence of rainfall forecast bias on model near surface relative humidity, which seems to relate to the handling of droplet evaporation and other cloud physics processes. All such errors can in principle be addressed via ECMWF’s “ecPoint” post-processing approach; indeed the conditional verification activity here was managed via ecPoint calibration software. The resulting corrections will be illustrated.

Whilst data-driven AI models are currently delivering better predictions of the synoptic pattern than classical physics-based global NWP, the fact remains that those AI models are generally using unadjusted re-analyses for training, and so the situation-dependant biases will clearly put a cap on skill attainable by them for surface weather parameters, even when the forecast synoptic pattern is ‘perfect’. Some ECMWF views on how to overcome this barrier, to deliver even better predictions, will be very briefly presented.

How to cite: Hewson, T.: Using Conditional Verification to describe Situation-dependant Model Biases for Surface Weather – Applications and Implications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18177, https://doi.org/10.5194/egusphere-egu25-18177, 2025.

This research aims to examine the evolution of the large-scale localized buoyancy anomalies in mid-latitude regions, investigating the adjustments in the atmosphere for moist-convective environments. For the global dynamical simulation, the two-layer moist-convective thermal rotating shallow water (mcTRSW) model Aeolus2.0 with intermediate complexity was employed. The concept of two interacting layers enabled the study of the dynamics of localized extreme heatwaves in baroclinic and barotropic situations. The model initialization comprises daily averaged velocity and potential temperature variables from ERA5 data. The results reveal the presence of a circular positive buoyancy anomaly in the lower layer, while the upper layer shows opposite circular rotation wind movement for some of the cases analyzed. The condensed liquid water content anomaly evolution shows that baroclinic localized buoyancy perturbation should play an important role for increased cloud formation and condensation, as a result of the heatwave propagation in the atmosphere for those extreme forcings. Comparing the strong and weak buoyancy anomalies results, we can notice the prolonged effects of baroclinic initial condition over the barotropic case.

How to cite: Oliveira Guimarães, S., Rostami, M., and Petri, S.: An Intermediate Complexity Approach to the Dynamics of Localized Extreme Heatwaves in the Mid-Latitude Atmosphere for moist-convective environments using Aeolus2.0, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18630, https://doi.org/10.5194/egusphere-egu25-18630, 2025.

EGU25-19296 | ECS | Posters on site | AS1.1

Assessing the Performance of Convection-Permitting Regional Climate Models in Simulating the 2002 Extreme Rainfall Event Over Central Europe 

Shruti Verma, Natalia Machado Crespo, Michal Belda, Tomas Halenka, Peter Huszar, and Eva Holtanova

Extreme rainfall events represent a substantial risk to regions across the globe, including the Central Europe. The 2002 Central European flood was a devastating natural disaster affecting countries like Germany, Austria, the Czech Republic, and Hungary. Intense rainfall, saturated soils, and overflowing rivers caused severe flooding, displacing many and leading to significant loss of life. With damages exceeding €20 billion, it remains one of Europe’s most costly flood events, heavily impacting historic cities such as Prague and Dresden (Chorynski et al., 2012).

The spatial and temporal resolution of climate models can present challenges when simulating extreme rainfall events at regional or local scales in term of both the intensity and spatial distribution of precipitation. Therefore, In this study the implementation of high-resolution RCMs with "explicit" convection has been applied which directly resolves deep convection on the model grid without relying on parameterization schemes, known as convection-permitting (CP) models (Prein et al., 2013a,b). This study evaluates the performance of RegCM5 in simulating two consecutive extreme rainfall events (6–7 and 11–13 August 2002) over Central Europe and the Czech Republic, comparing 12 km and 3 km i.e. CP-RCM simulations along with sensitivity of planetary boundary layer (PBL) scheme Holtslag and UW. The results reveal significant discrepancies in the 12km RCM simulations, particularly in Czech Republic, where they struggle to capture the rainfall patterns of both events. The model configurations with UW PBL closely follow the observed extreme rainfall patterns, demonstrating improved alignment with the events. While CP simulations improve the representation of small-scale processes, accurately capturing localized extreme events, particularly the first spell, remains challenging. These findings highlight the potential of CP-RCM simulations for extreme precipitation in terms of climate adaptation, infrastructure development, and policy planning to mitigate the potential risks

How to cite: Verma, S., Crespo, N. M., Belda, M., Halenka, T., Huszar, P., and Holtanova, E.: Assessing the Performance of Convection-Permitting Regional Climate Models in Simulating the 2002 Extreme Rainfall Event Over Central Europe, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19296, https://doi.org/10.5194/egusphere-egu25-19296, 2025.

EGU25-19431 | ECS | Orals | AS1.1

Anemoi: A New Collaborative Framework for Data-driven Weather Forecasting 

Ana Prieto Nemesio, Daniele Nerini, Jasper Wijnands, Thomas Nipen, and Matthew Chantry

Anemoi is an open-source framework co-developed by ECMWF and several European national meteorological services to build, train, and run data-driven weather forecasts. Its primary goal is to empower meteorological organisations to train machine learning (ML) models using their data, simplifying the process with shared tools and workflows.
Designed for modularity and flexibility, Anemoi offers key components for efficient data-driven forecasting. The framework is organised into distinct Python packages covering the entire machine learning lifecycle—from the creation of customised datasets from diverse meteorological sources to the development and training of advanced deep learning graph models. Once a model is trained, Anemoi enables users to run it for inference, using the outputs of physics-based NWP analyses or ensembles as initial conditions, while maintaining comprehensive lineage tracking.
Anemoi has already been applied in experimental operational forecasting, including ECMWF’s Artificial Intelligence Forecasting System (AIFS). It has supported models utilising stretched grid and limited-area configurations. These applications demonstrate Anemoi’s potential to enhance forecasting accuracy by integrating ML techniques into existing systems.
More than just a technical framework, Anemoi represents a collaborative effort among meteorological services, researchers, and technologists, fostering knowledge exchange and innovation.

How to cite: Prieto Nemesio, A., Nerini, D., Wijnands, J., Nipen, T., and Chantry, M.: Anemoi: A New Collaborative Framework for Data-driven Weather Forecasting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19431, https://doi.org/10.5194/egusphere-egu25-19431, 2025.

EGU25-19706 | Posters on site | AS1.1

Advances in Project IMA, the Seamless Prediction Programme of the Royal Meteorological Institute of Belgium 

Lesley De Cruz, Simon De Kock, Michiel Van Ginderachter, Maarten Reyniers, Alex Deckmyn, Idir Dehmous, Wout Dewettinck, Felix Erdmann, Ruben Imhoff, Arthur Moraux, Ricardo Reinoso-Rondinel, Mats Veldhuizen, Joseph James Casey, Loic Faleu Kemajou, Anshul Kumar, and Viktor Van Nieuwenhuize

Seamless prediction systems provide frequently updated forecasts across different timescales by combining observations, such as weather radar data, with numerical weather prediction (NWP) models. These systems are increasingly needed by users like hydrological services, local authorities, renewable energy operators, and smartphone apps to make better and earlier decisions. This is especially true for precipitation, which is highly variable in space and time and strongly influences downstream models like (urban) hydrology. To achieve this, forecasts must not only be fast and accurate but also come with calibrated ensembles to estimate uncertainty and propagate errors properly.
In Belgium, Project IMA (inspired by the Japanese word for "now" or "soon") is the seamless prediction system developed by the Royal Meteorological Institute (RMI). It uses RMI’s observation network, including RADQPE for gauge-corrected precipitation estimates, the pysteps-be probabilistic rainfall nowcasting system, the INCA-BE nowcasting system, and the ACCORD NWP models ALARO and AROME. Unlike many other systems, Project IMA offers seamless ensemble precipitation nowcasts for lead times up to 6 hours, updated every 5 minutes, designed to improve flash flood predictions and quantify their uncertainty.
This presentation will showcase recent developments in Project IMA, including updates to the open-source pysteps framework, such as an improved runtime efficiency, code structure and better representation of extremes. We will discuss new deep learning-based methods for blending forecasts to extend their lead time and improve accuracy, calibration, and usefulness for end users such as hydrologists, crisis managers and water authorities.
Project IMA aims to ensure a rapid transfer from research to operations and encourages open-source contributions to ensure transparency and reproducibility. It supports the United Nations’ “Early Warnings for All” initiative, which strives to make forecasts more accessible and actionable by 2027.

How to cite: De Cruz, L., De Kock, S., Van Ginderachter, M., Reyniers, M., Deckmyn, A., Dehmous, I., Dewettinck, W., Erdmann, F., Imhoff, R., Moraux, A., Reinoso-Rondinel, R., Veldhuizen, M., Casey, J. J., Faleu Kemajou, L., Kumar, A., and Van Nieuwenhuize, V.: Advances in Project IMA, the Seamless Prediction Programme of the Royal Meteorological Institute of Belgium, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19706, https://doi.org/10.5194/egusphere-egu25-19706, 2025.

Accurate weather forecasting is vital for societal decision-making in sectors such as renewable energy, agriculture, and disaster management. Statistical post-processing techniques play a critical role in calibrating forecasts and addressing issues of model bias and ensemble dispersion. However, many post-processing methods rely on complete and high-quality datasets, and the presence of missing data can significantly undermine their effectiveness. This study presents a comparative analysis of imputation methods aimed at bridging data gaps to enhance the performance of statistical post-processing techniques.
The evaluation process focuses on a selection of widely used imputation approaches, including ensemble member mean substitution, persistence, Fourier fit, and Neural Networks. These methods are assessed using the forecasts and observations from the EUPPBench dataset by introducing randomly selected missing data, focusing on metrics such as imputation accuracy and their impact on post-processing performance. To quantify the benefit of missing data imputation the study compares different post-processing techniques, ranging from the simpler EMOS to the more advanced Neural Networks, where the latter is known to be more affected by incomplete data. 

How to cite: Lakatos-Szabó, M.: A comparative study of imputation methods for improving statistical post-processing of weather forecasts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19873, https://doi.org/10.5194/egusphere-egu25-19873, 2025.

The Asian Summer Monsoon Anticyclone (ASMA) plays a critical role in trapping, transporting, and redistributing water vapour in the upper troposphere and lower stratosphere, particularly into the extratropical lower stratosphere. Comparison of ERA5 reanalysis data with remote sensing data and simulations with the model ICON-CLM in convection-parameterized (12 km grid spacing) and convection-permitting (3.3 km) setups indicate that the transport into the ASMA is overestimated in ERA5 over the Tibetan plateau (Singh & Ahrens 2023). This presentation critically discusses the water vapour transport into the upper-troposphere/lower-stratosphere by deep convective events over the Tibetan plateau and the Himalayas – an area identified as hotspot for troposphere-stratosphere exchange (Škerlak et al. 2014) using convection-parameterized reanalysis data. Our investigations use a decade-long ICON-CLM climate-like simulation (Collier et al. 2024) performed as a contribution to the CORDEX flagship pilot study Convection-Permitting Third Pole (CPTP).

References

Collier, E., N. Ban, N. Richter, B. Ahrens, D. Chen, X. Chen, H-W. Lai, R. Leung, L. Li, T. Ou, P.K. Pothapakula, E. Potter, A. F. Prein, K. Sakaguchi, M. Schroeder, P. Singh, S. Sobolowski, S. Sugimoto, J. Tang, H. Yu, C. Ziska: The First Ensemble of Kilometre-Scale Simulations of a Hydrological Year over the Third Pole. Clim Dyn. https://doi.org/10.1007/s00382-024-07291-2, 2024

Singh, P., B. Ahrens: Modeling Lightning Activity in the Third Pole Region: Performance of a km-Scale ICON-CLM Simulation. Atmosphere, 14(11), 1655, DOI: 10.3390/atmos14111655, 2023

Škerlak, B., M. Sprenger, and H. Wernli: A global climatology of stratosphere–troposphere exchange using the ERA-Interim data set from 1979 to 2011. English. Atmospheric Chemistry and Physics 14 (2), 913–937. doi: 10.5194/acp-14-913-2014, 2014

How to cite: Ahrens, B. and Singh, P.: Moist convection and tracer transport in and out of the Asian Summer Monsoon Anticyclone, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20360, https://doi.org/10.5194/egusphere-egu25-20360, 2025.

EGU25-21081 | ECS | Posters on site | AS1.1

Spatial and Temporal Verification of High-Resolution Modelled Rainfall Data for Urban Flood Risk Assessment 

Markus Pichler and Dirk Muschalla

Reliable climate forecasts are crucial for adapting to future challenges, particularly in urban flood management, where pluvial flooding poses a significant threat. This study focuses on the verification and enhancement of rainfall data for urban flood modelling by analysing critical aspects such as total depth, intensities, seasonality, dry weather periods, and spatial distribution during extreme storm events.

In Graz, Austria, a network of 23 high-resolution precipitation measurement stations covering 120 km², including 13 stations with over a decade of data, was utilized to calibrate a regional climate model through a downscaling approach. This provided minute-level rainfall data for each station, enabling a detailed comparison of historical measurements from the past 10 years with climate model outputs for the current state of the climate. Subsequently, changes in key rainfall characteristics were assessed for the near future (2040–2050) and far future (2090–2100).

Our analysis evaluated yearly precipitation totals, spatial rainfall distribution, intensity-duration-frequency (IDF) functions, and the seasonality of extreme rainfall events. The results revealed promising alignment with historical data, though discrepancies were noted for shorter durations and seasonal shifts. Specifically, heavy rainfall events were projected to occur more frequently in autumn in the future, a trend absent in historical observations.

This study underscores the importance of statistically robust downscaling and verification techniques in blending observational and model-based forecasts to enhance the reliability of climate predictions. These advancements provide critical insights for urban flood resilience planning and illustrate the evolving nature of extreme rainfall under changing climatic conditions.

How to cite: Pichler, M. and Muschalla, D.: Spatial and Temporal Verification of High-Resolution Modelled Rainfall Data for Urban Flood Risk Assessment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21081, https://doi.org/10.5194/egusphere-egu25-21081, 2025.

EGU25-3861 | Posters on site | CL4.11

Advancing Climate System Understanding: Insights from the PalMod Project 

Kerstin Fieg, Mojib Latif, Michael Schulz, and Tatiana Ilyina

The PalMod project, funded by the German Federal Ministry of Education and Research (BMBF), aims at addressing key knowledge gaps in the understanding of the dynamics and variability of the climate system during the last glacial cycle. This period, which is marked by strong and rapid climatic fluctuations, serves as a testbed for complex Earth system models (ESMs). The models tested in this way will be used in climate-change scenarios for the next millennia to enhance future climate-change assessments. PalMod uses three ESMs—AWI-ESM, MPI-ESM, and CESM— that integrate physical and biogeochemical processes and employ advanced parameterizations regarding, for example, ice sheet-ocean interactions.

In Phases I and II, the project focused on key epochs of the last glacial cycle including inception, MIS3, and the last deglaciation. The ongoing final Phase III leverages these insights to project the climate over the next millennia. Central to this last project phase is to answer some of the major societally critical questions in association with climate change: What are the potential tipping points and at which global warming may they become relevant? Under what conditions could polar ice sheets collapse catastrophically, and how rapidly could sea levels rise under different future climate scenarios? How will permafrost evolve in a warming world? This presentation reflects on the progress made during the past two phases of the project and presents preliminary answers to the aforementioned pressing questions.

How to cite: Fieg, K., Latif, M., Schulz, M., and Ilyina, T.: Advancing Climate System Understanding: Insights from the PalMod Project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3861, https://doi.org/10.5194/egusphere-egu25-3861, 2025.

EGU25-4864 | Posters on site | CL4.11

Convection Permitting Regional Paleoclimate Simulations with Climate-Driven Land-Use Mapping for a reduced Mediterranean domain 

James Ciarlo`, Arthur Lamoliere, Graziano Giuliani, Erika Coppola, Aaron Micallef, and David Mifsud

The Central Mediterranean's complex topography and dynamic land-sea interactions provide a compelling opportunity for high-resolution paleoclimate modelling aimed at enhancing our understanding of natural climate variability. This study utilizes the RegCM5 regional climate model to conduct km-scale simulations, focusing on fine-scale climate dynamics for a reduced Mediterranean domain across five pivotal paleoclimate periods: Modern (ca. 1995 CE), Pre-Industrial (ca. 1850 CE), Medieval Climate Anomaly (MCA, ca. 1000 CE), mid-Holocene (6000 BP), and Last Glacial Maximum (LGM, 21000 BP). Simulations are driven by MPI-ESM-LR model outputs from PMIP4, with ERA5 reanalysis data used for evaluation runs.

A novel land-use mapping technique is applied, leveraging Köppen-Geiger climate classifications and current vegetation distributions to reconstruct paleoclimate vegetation patterns. Simulation results are benchmarked against E-OBS, ModE-RA, MCruns, and lgmDAnomaly datasets, revealing typical biases. Historical data exhibits a cold bias, while the 6000 BP period shows scattered low-level wet and cold biases, and the 21000 BP period presents warm and wet biases. Despite these challenges, the km-scale simulations effectively capture detailed climatic patterns, providing crucial insights into the Mediterranean’s paleoclimate and regional implications. These findings highlight the value of downscaling global models to km scales, which can advance our understanding of past climate dynamics and informing strategies for future climate adaptation.

How to cite: Ciarlo`, J., Lamoliere, A., Giuliani, G., Coppola, E., Micallef, A., and Mifsud, D.: Convection Permitting Regional Paleoclimate Simulations with Climate-Driven Land-Use Mapping for a reduced Mediterranean domain, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4864, https://doi.org/10.5194/egusphere-egu25-4864, 2025.

EGU25-5445 | ECS | Posters on site | CL4.11

Arctic river blockage and the formation of glacial deep ocean salinity anomalies  

Hyuna Kim, Axel Timmermann, and Miho Ishizu

Substantial snow accumulation over northern continents during glacial periods contributed to the growth of the Laurentide and Eurasian ice sheets. As a result sea level dropped by ~120-130 m, which led to an increase in global mean ocean salinity by about 1 permil. Pore water chlorinity data from deep ocean sediment cores interestingly show even higher values regionally. Despite this superficial understanding of glacial ocean salinity shifts, the three-dimensional patterns of paleosalinity changes are still not well understood. Here, we argue that northern hemisphere ice-sheets effectively blocked pan-Arctic river discharge into the Arctic Ocean for millennia. In the absence of ice-sheet calving and melting, this process was responsible for the gradual accumulation of the 1 permil global mean salinity anomaly during glacial periods. To better understand the underlying physical mechanisms, we use the Community Earth System Model and mimic the freshwater withholding of the ice-sheets as an idealized negative freshwater perturbation. Applying this forcing scenario, we find that the river blockage due to the Laurentide and Eurasian ice-sheets removes the polar halocline, strengthens the Atlantic Meridional Overturning Circulation and contributes to the global increase of salinity at a rate of 0.1 permil/1000 years. Moreover, the process creates a characteristic pattern of deep ocean salinity anomalies, which is distinct from the vertical salinity redistribution due to sea-ice/brine formation in the Southern Ocean. Eventually, for glacial conditions both, the Arctic and Southern Ocean-generated salinity patterns combine.

How to cite: Kim, H., Timmermann, A., and Ishizu, M.: Arctic river blockage and the formation of glacial deep ocean salinity anomalies , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5445, https://doi.org/10.5194/egusphere-egu25-5445, 2025.

EGU25-6568 | ECS | Orals | CL4.11

Using Past Surface Water Density to Constrain Future South Asian Monsoon Precipitation 

Héloïse Barathieu, Thibaut Caley, Valentin Portmann, Didier Swingedouw, Masa Kageyama, Pascale Braconnot, Didier Roche, Niclas Rieger, Bruno Malaizé, Marion Peral, Emilie Dassié, Karine Charlier, and Franck Bassinot

The hydrological cycle plays a crucial role in the Earth’s climate and has a direct impact on human populations. Despite advances, the IPCC AR6 report highlights persistent uncertainties concerning future projections of potential changes in the hydrological cycle, in particular for low latitudes monsoonal systems. This is because numerical climate models exhibit significant spread in their projections.

Traditionally, to estimate the future value of a climate variable, the distribution of projections from an ensemble of models is examined. However, this uncertainty is very high for water cycle, and the best estimates may be biased. To improve these projections, observational constraint, or emergent constraint methods, have been developed. These approaches adjust the distribution of projected variables based on observations, helping to reduce uncertainty. Furthermore, some studies show that the spatial pattern of sea surface salinity (SSS) is strongly correlated with the mean spatial pattern of the evaporation-precipitation (E-P) balance. Given that, water surface density is mainly influenced by salinity changes in region with strong precipitation and coastal runoff, both salinity and density could provide a useful tracer of the hydrological cycle.

In this study, we reconstruct past sea surface density based on geochemical analyses (ẟ18Oc) on foraminifera extracted from marine sediment cores in the Bay of Bengal. Density changes in this dilution basin are mainly related to south Asian monsoon precipitation changes. We used our density reconstructions for the last glacial maximum (LGM) and Mid-Holocene (MH) as a predictor for the observational constraint method. Our goal is to reduce uncertainties in future South Asian monsoon precipitation projections in climate models by linking paleoclimatic information with future climate projections. To do so, we used PMIP and CMIP numerical climate modelling experiments.

Our preliminary results show an underestimation of South Asian monsoon precipitation in the future (2000-2100) in most models, when using historical surface density and salinity (1900-2000) as a predictor. We are currently finalizing the use of LGM and MH surface density as predictor, in order to compare results when past predictors (LGM and MH) are used rather than an historical predictor.

How to cite: Barathieu, H., Caley, T., Portmann, V., Swingedouw, D., Kageyama, M., Braconnot, P., Roche, D., Rieger, N., Malaizé, B., Peral, M., Dassié, E., Charlier, K., and Bassinot, F.: Using Past Surface Water Density to Constrain Future South Asian Monsoon Precipitation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6568, https://doi.org/10.5194/egusphere-egu25-6568, 2025.

A rapid change in the Atlantic overturning circulation (AMOC) can have a major impact on the hydrological cycle over land and ecosystems. Examples of such events have been widely discussed in palaeoclimate studies investigating the response of the AMOC to rapid freshening of the North Atlantic caused by ice sheet instability and melting during ice ages or in the early Holocene (Wunderling et al. 2024). The rapid decline of the AMOC and the possibility of its collapse in the future could also have a major impact on terrestrial ecosystems. An open question is the identification of precursors to such shifts and the anticipation of impacts and feedbacks on ecosystems. Here we use as a starting point a transient simulation of the last 6 000 years with version IPSLCM6-LR of the IPSL model (Boucher et al. 2020), starting from the PMIP mid-Holocene simulation with this model (Braconnot et al. 2021).  Surprisingly, this simulation shows a rapid shift of 2 Sv in the AMOC, while this type of bifurcation was not seen in the set of CMIP6 simulations run with the same version of the model. (Boucher et al. 2020). Such a shift doesn't occur in a parallel simulation using a slightly different version of the model with fully interactive vegetation. The presentation will discuss the set of simulations used to identify 1) the reason for the shift, 2) the impact of the shift on the vegetation in Africa and Europe. For the latter, we run snapshot coupled simulations using as initial state the ocean state of the Holocene simulation with the AMOC shift, and the corresponding Earth’s orbit and trace gas configuration.  This allows us to estimate the amplification of the changes induced by the vegetation feedback on the regional changes in the hydrological cycle. 

 

Boucher O, Servonnat J, Albright AL, et al (2020) Presentation and Evaluation of the IPSL-CM6A-LR Climate Model. J Adv Model Earth Syst 12:e2019MS002010. https://doi.org/10.1029/2019ms002010

Braconnot P, Albani S, Balkanski Y, et al (2021) Impact of dust in PMIP-CMIP6 mid-Holocene simulations with the IPSL model. Clim Past 17:1091–1117. https://doi.org/10.5194/cp-17-1091-2021

Wunderling N, Von Der Heydt AS, Aksenov Y, et al (2024) Climate tipping point interactions and cascades: a review. Earth Syst Dyn 15:41–74. https://doi.org/10.5194/esd-15-41-2024

How to cite: Braconnot, P. and Marti, O.: Rapid change in AMOC intensity in a Holocene transient simulation provides insight into the ocean long term ocean memory  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7053, https://doi.org/10.5194/egusphere-egu25-7053, 2025.

EGU25-8946 | ECS | Posters on site | CL4.11

Impact of Past AMOC Disruptions on Ocean Oxygenation  

Eva M. Rückert, Bo Liu, and Tatiana Ilyina

The global ocean plays a crucial role in redistributing and storing heat, carbon, nutrients and other essential elements in the Earth’s climate system. As a prominent part of the global ocean circulation, the Atlantic Meridional Overturning Circulation (AMOC) shapes the spatial distribution of these elements and links the atmosphere to the deep ocean.

The state of ocean oxygenation and the carbon storage capacity are tightly connected to biogeochemical activity. High oxygen levels facilitate the efficient remineralization of organic matter, helping to stabilize the CO2 content in the upper ocean layers. In contrast, low oxygen levels enhance carbon storage in the deep ocean temporarily but increase the risk of pronounced outgassing during ocean circulation changes or upwelling events. Thus, ocean oxygenation acts both as an indicator and a control on biogeochemistry and thus long-term climate regulation.

Proxy data indicate substantial changes in AMOC strength in the past, particularly during Termination 1, when high freshwater fluxes disrupted deep water formation and significantly slowed down the ocean circulation. Despite these insights, the interplay between changes in ocean circulation, oxygenation and carbon storage and release during such abrupt events is still not fully understood.

To address these knowledge gaps, we used the Max Planck Institute for Meteorology Earth system model (MPI-ESM) coupled with the interactive Hamburg ocean carbon cycle model (HAMOCC) to simulate transient climate changes during the last deglaciation.

We focused on periods of major AMOC disruptions during the last deglaciation to investigate their impact on the ocean’s oxygen levels in the water column.

Preliminary results indicate a delayed increase of the global oxygen minimum zone (OMZ) volume following abrupt AMOC changes. The most significant changes in the oxygen levels can be observed in the Atlantic Sector of the Southern Ocean. Additionally, we explore the feedbacks between changes in oxygenation, carbon storage, and biological activity across these events.

This research provides new insights into the complex interplay between ocean circulation, oxygen dynamics, and carbon storage during deglacial periods, advancing our understanding of the mechanisms underlying abrupt climate events and their biogeochemical impacts.

How to cite: Rückert, E. M., Liu, B., and Ilyina, T.: Impact of Past AMOC Disruptions on Ocean Oxygenation , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8946, https://doi.org/10.5194/egusphere-egu25-8946, 2025.

The ocean carbon sink and deoxygenation are two key research focuses under the current anthropogenically warming climate, as the former is essential in regulating atmospheric CO2, and the latter is a vital factor for the marine ecosystem. The oceanic carbon and oxygen cycles are closely linked as they are commonly influenced by several processes, such as temperature-dependent gas solubility, organic matter remineralisation in the interior ocean, and ventilation. Future predictions of ocean carbon sink and deoxygenation are still subject to considerable uncertainties as the observational data in the present-day ocean is too sparse to constrain the relevant natural processes. To deepen our understanding of the natural carbon and oxygen cycles, we use the state-of-the-art Max Planck Institute Earth System Model (MPI-ESM) to conduct transient simulations for the last deglaciation (21 ka to the present day).

The deglacial evolution of oceanic CO2 outgassing is mainly controlled by gradual global warming and the Atlantic Meridional Overturning Circulation (AMOC) variability driven by the meltwater from the prescribed ice sheet reconstruction. The global ocean oxygen content generally captures the features of the qualitative oxygen proxies, with lower oxygen content in the glacial ocean compared to the Holocene and a decrease in global oxygen content as the AMOC declines. The low oxygen content in the glacial ocean results from lower oxygen content in the deep ocean (below 2000 m), which is partially counteracted by higher oxygen content in the upper ocean, owing to solubility increase under colder temperatures. The glacial deep-ocean deoxygenation is governed by the air-sea disequilibrium under a more extensive, longer-lasting sea ice cover in the Southern Ocean and a more sluggish transport between the upper and interior ocean. Unlike the ocean carbon content, which closely follows the temporal variation of the North Atlantic Deep Water (NADW) strength, the evolution of the oxygen content is slow and decoupled from the NADW during its recovery phase, suggesting the Southern Ocean ventilation has a more significant impact on the oxygen dynamics. For the mid and late Holocene, when the ocean circulation is quasi-stable, the global air-sea CO2 flux is near zero, whereas the replenishment of deep-sea oxygen continues. Such different response time scales between the ocean carbon and oxygen cycles are also seen in additional sensitivity simulations where an AMOC decline and recovery are simulated by freshwater hosing. Our preliminary findings suggest that the past changes in the climate and ocean circulation are likely to have a long-lasting impact on oxygen dynamics and drive oxygen concentrations away from equilibrium states, which should be accounted for when conducting model-data comparisons.

How to cite: Liu, B., Rückert, E., and Ilyina, T.: Different time scales in the transient response of the ocean carbon and oxygen cycles to deglacial climate change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11435, https://doi.org/10.5194/egusphere-egu25-11435, 2025.

EGU25-11848 * | ECS | Orals | CL4.11 | Highlight

North American forest dieback simulated in response to warm mid-Holocene summers 

Alfred J. Wilson, Peter O. Hopcroft, Anya J. Crocker, Richard G. Stockey, Charles J. R. Williams, and Paul A. Wilson

Vegetation plays a critical role in regulating climate, not least as a sink of atmospheric carbon. How will anthropogenic warming affect the future distribution and behaviour of vegetation? The study of past warm intervals can contextualise biosphere responses to changes in temperature and precipitation. Pollen archives from central North America, in the Great Plains region, suggest that mid-Holocene (10-4 ka) warming was characterized by an abrupt expansion of grasslands and reduced forest cover. It has been suggested that these changes were a response to drying triggered by an increase in insolation and the abrupt collapse of the Laurentide Ice Sheet but evidence in support of this explanation is lacking. Here we report results from a new dynamic vegetation simulation of the mid-Holocene (6 ka) using the United Kingdom Earth System Model version 1.1 (UKESM1.1), in an atmosphere-land-only configuration. Our simulation is forced by sea-surface temperatures and sea-ice concentrations derived from the PMIP4 HadGEM3-GC3.1 midHolocene experiment and the orbit and greenhouse gas concentrations follow the PMIP4 protocol. In response to summer warming of between 0.5 and 1.5 °C, the model simulates a drying of up to 200 mm yr-1 in the North American continental interior and a substantial decrease in soil moisture. These land surface changes drive shifts in the distribution of plant functional types (PFTs) with a widespread decline in the fractional coverage of forests and a concurrent expansion of grasslands. The forest dieback is most intense in the north and central US and Canadian Great Plains where coverage falls by an area roughly equivalent to half the size of Texas.  

How to cite: Wilson, A. J., Hopcroft, P. O., Crocker, A. J., Stockey, R. G., Williams, C. J. R., and Wilson, P. A.: North American forest dieback simulated in response to warm mid-Holocene summers, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11848, https://doi.org/10.5194/egusphere-egu25-11848, 2025.

EGU25-12057 | ECS | Posters on site | CL4.11

Transient climate simulation of the past 4.5 million years based on the coupled intermediate complexity model iLOVECLIM 

Thomas Extier, Alicia Hou, Thibaut Caley, Didier M. Roche, Peter Köhler, and Roderik S. W. van de Wal

The Earth experienced dramatic climate changes during the past million years, including a long-term gradual cooling from the Pliocene (5.3-2.6 million years ago; Ma) to the Pleistocene (2.6-0.011 Ma) and an abrupt transition from 41-kyr to 100-kyr glacial-interglacial cycles at ca. 1.2-0.8 Ma (i.e., the Mid-Pleistocene transition). Investigating the mechanisms that triggered these climatic responses requires long-term transient climate simulations which can be used to quantify the sensitivity of the Earth’s climate to different external and internal forcings. However, few such simulations exist and therefore, key questions regarding the long-term evolution of the earth system remain unanswered.

Here, we used iLOVECLIM, a coupled Earth system numerical climate model of intermediate complexity, to generate a 4.5 Ma transient climate simulation, the longest to date. iLOVECLIM is ideally suited for this task as it requires substantially less computational resources and time to perform transient climate simulations compared to fully coupled general circulation models. We performed the simulations with interactive atmosphere, ocean and vegetation components and used the methodology of previous long-term transient simulations. Briefly, we applied an acceleration factor of five to the external forcings (orbital parameters, greenhouse gases concentration and ice-sheets) and split the 4.5 Ma simulation into 44 chunks run in parallel to reduce the computing time from several years to a couple of months. Each chunk was initialized from an interglacial period, covers at least one glacial-interglacial cycle and has an overlap period of 20,000 years in order to compensate for issues related to spin-up effects and initial conditions. The complete simulation is a composite of all the individual chunks and time-sliding linear interpolation performed on the overlap intervals.

While the simulations are still ongoing, preliminary results demonstrate that our new model set-up and experimental design are able to produce reasonable outputs. When it is completed, the final simulation will be evaluated against available paleoclimate data and existing transient climate simulations. Apart from running a simulation with all the external forcings combined, we also plan to run subsequent simulations with each individual forcing alone to evaluate the climate responses associated with each. This unique long transient simulation will provide a better mechanistic understanding of the major climate reorganizations that occurred during the Plio-Pleistocene and will be useful for future data-model comparisons and data assimilation endeavours.

How to cite: Extier, T., Hou, A., Caley, T., Roche, D. M., Köhler, P., and van de Wal, R. S. W.: Transient climate simulation of the past 4.5 million years based on the coupled intermediate complexity model iLOVECLIM, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12057, https://doi.org/10.5194/egusphere-egu25-12057, 2025.

EGU25-13365 | Orals | CL4.11

Sensitivity of the Pliocene Climate to CO2, Orbital Forcing and Vegetation.  

Julia Tindall, Alan Haywood, and Stephen Hunter

The climate of the Late Pliocene (3.60-2.58Ma), has been extensively studied using models and data, as it represents the most recent period in Earth history where CO2 levels were similar to the present day.   Within this interval, Marine Isotope Stage (MIS) KM5c (~3.205Ma) also had similar to present day orbital configuration, and hence was the subject of the second phase of the Pliocene Modelling Intercomparison Project (PlioMIP2). 

Phase 3 of PlioMIP (PlioMIP3) is now underway and includes a number of sensitivity experiments to assess how the Late Pliocene climate would have been expected to respond to different CO2 levels (280ppmv, 400ppmv, 490ppmv and 560ppmv), extreme orbits and vegetation.   

Here we will present results from these sensitivity experiments, which have been run using the Hadley Centre Climate Model (HadCM3).  We find that the CO2  changes have a slightly smaller effect on temperatures when using Late Pliocene boundary conditions, than when using preindustrial, however the differences are region dependent.  For example, Southern Ocean warming due to CO2 is notably lower with Pliocene boundary conditions than with preindustrial.  This is partly because non-CO2 Pliocene forcing has already warmed this region significantly, however non-linearities will be discussed.  

Results from the Late Pliocene experiment with a warm northern hemisphere summer orbit, and a warm southern hemisphere summer orbit will also be presented.  This will allow us to assess how temperature and precipitation patterns could have varied throughout the Late Pliocene.   The relative importance of paleogeography changes, CO2 changes, orbital changes and vegetation changes on Pliocene warming will be analysed.  

 

How to cite: Tindall, J., Haywood, A., and Hunter, S.: Sensitivity of the Pliocene Climate to CO2, Orbital Forcing and Vegetation. , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13365, https://doi.org/10.5194/egusphere-egu25-13365, 2025.

EGU25-13628 | ECS | Posters on site | CL4.11

Modeling Paleocene-Eocene Hyperthermals with the PlaSim-LSG Earth System Model of Intermediate Complexity 

Isabella Ghirardo and Jost Hardenberg

Hyperthermal events, such as the Paleocene-Eocene Thermal Maximum (PETM, 56 million years ago) and Early Eocene Climatic Optimum (EECO, 52 million years ago), are of significant interest because they offer critical insights into how the Earth’s climate reacts to rapid increases in greenhouse gas concentrations. These events, marked by intense global warming and ocean acidification, improve our understanding of the long-term effects of sudden carbon releases and help assess the potential impacts of today's human-driven climate change.

In this study, we use a version of the Planet Simulator (PlaSim), an Earth Model of Intermediate Complexity (EMIC) improved with a 3D ocean model (Large-Scale Geostrophic ocean model, LSG), to simulate these hyperthermal periods. This modeling approach allows for detailed analyses of ocean-atmosphere interactions and their role in shaping global climate patterns under extreme GHG scenarios. The simulations include boundary conditions derived from Herold et al. (2014) and use an experimental approach similar to the DeepMIP protocol. We explore a range of atmospheric CO2 levels (from 1× to 16× pre-industrial concentrations) to evaluate the sensitivity of the climate system to these factors.

The focus is on understanding feedback mechanisms and climate dynamics under extreme greenhouse gas forcing, while also considering equilibrium climate sensitivity (ECS) and polar amplification, with attention to Antarctic warming and its implications for ice-free conditions during the late Paleocene–early Eocene. Current work involves testing and refining paleoclimate boundary conditions in the Planet Simulator, particularly adjusting paleogeography, vegetation parameters, and ocean circulation to match the climate conditions of that period. This study improves our understanding of past extreme greenhouse climates and evaluates the ability of modern Earth System Models (ESMs) to predict future climate changes.

How to cite: Ghirardo, I. and Hardenberg, J.: Modeling Paleocene-Eocene Hyperthermals with the PlaSim-LSG Earth System Model of Intermediate Complexity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13628, https://doi.org/10.5194/egusphere-egu25-13628, 2025.

EGU25-13785 | Orals | CL4.11

Experimental design for DeepMIP-Eocene Phase 2 - impact of new paleogeography and vegetation 

Dan Lunt and the The DeepMIP-Eocene Team

Warm, high-CO2 climates of Earth's past provide an opportunity to both evaluate climate models under extreme forcing and to explore mechanisms that lead to such warmth.  One such time period is the early Eocene, when global mean surface temperatures were 10-16 oC higher than preindustrial, and  CO2 concentrations were about ~1500 ppmv.

In this presentation we present the experimental design for Phase 2 of the Eocene component of the Deep-time Model Intercomparison project (DeepMIP-Eocene-p2).  The aim is to provide a framework within  which modelling groups can carry out a common set of simulations, thereby facilitating exploration of inter-model dependencies.  Focus is on the early Eocene Climatic Optimum (EECO, ~53.3-49.1 million years ago).  Relative to Phase 1 of DeepMIP, we provide a new paleogeography (topography, bathymetry) derived from four independent reconstructions, a new vegetation derived from vegetation model simulations that have been evaluated with paleobotanical data, and a new CO2 specification derived from the boron isotope proxy.  The core set of simulations consists of a preindustrial control, an abrupt increase to 4x preindustrial CO2 concentrations under modern conditions, a standard control EECO simulation at 5x preindustrial CO2 concentrations, and an EECO simulation with preindustrial CO2 concentrations.  In addition to these core simulations, we suggest a suite of optional sensitivity studies, which allow various sensitivities to be explored, such as to topography/bathymetry, greenhouse gases, land-surface parameters, astronomical and solar forcings, and internal model parameters.  Overall, we hope that the updated boundary conditions and guidance on initialisation in Phase 2 will allow more robust model-data comparisons, more accurate insights into mechanisms influencing early Eocene climate, and increased relevance for informing future climate change projection. 

In addition to the exprimental design, we present intitial simulations with the HadCM3 model with the new boundary conditions, and compare with the results from Phase 1, illustrating the sensitivity to the new paleogeography and vegetation.

 

How to cite: Lunt, D. and the The DeepMIP-Eocene Team: Experimental design for DeepMIP-Eocene Phase 2 - impact of new paleogeography and vegetation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13785, https://doi.org/10.5194/egusphere-egu25-13785, 2025.

EGU25-13793 | ECS | Posters on site | CL4.11

Ocean surface wind variability under the Pliocene warmth 

Hana Kawashima and Shineng Hu

During the mid-Pliocene, carbon dioxide (CO2) concentrations were comparable to current levels, ~350-450 p.p.m., making the mid-Pliocene a valuable analog for current and potentially future climates. However, the global average temperature in the mid-Pliocene is estimated to have been ~3 ºC higher than today, implying factors beyond greenhouse gases contributed to the warmth. Surface wind velocity, a key driver of ocean mixing and air-sea turbulent heat flux, significantly affects ocean heat content and global heat distribution. Understanding the role of surface wind speed in warm climates is therefore important to uncover the causes of the Pliocene warmth. 

In this study, we utilized a set of climate models from the Coupled Model Intercomparison Project (CMIP) and the Paleoclimate Modeling Intercomparison Project (PMIP) archives to analyze surface wind variability in the tropics during the mid-Pliocene and the Pre-industrial periods. Over the tropics, surface wind velocity is strongly influenced by sea surface temperature (SST) patterns, predominantly El Niño-Southern Oscillation. To explore the underlying mechanisms of surface wind variability, we applied Empirical Orthogonal Functions (EOF) to tropical SST data to extract SST patterns and decompose surface wind speed into SST-dependent and SST-independent components. Our results revealed that the ratio of SST-dependent and SST-independent wind variability could vary substantially in space and with season, and it could differ between the mid-Pliocene and the Pre-industrial period with a large inter-model spread. Implications for understanding the mid-Pliocene warmth and constraining future climate projection will be discussed.

How to cite: Kawashima, H. and Hu, S.: Ocean surface wind variability under the Pliocene warmth, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13793, https://doi.org/10.5194/egusphere-egu25-13793, 2025.

EGU25-14091 | Orals | CL4.11

A brief note on Supercooled Glacial Deep Waters 

Miho Ishizu, Axel Timmermann, and Yun Kyung-Sook

According to hydrographic profiles, about 2-5% of the present deep Southern Ocean waters have temperatures below the freezing point. Which role these supercooled waters may have played under glacial conditions is an open question. To elucidate the variations and mechanisms of deep ocean supercooling in the past we analyze a recently conducted quasi-transient earth system model simulation (CESM1.2), which covers the climate history of the past 3 million years. After the mid-Pleistocene Transition (MPT, ~1.2-0.75 million years ago, Ma) the simulation shows the presence of substantial volumes of supercooled glacial intermediate/deep waters primarily in the equatorial to northern Pacific. Our study explores the formation mechanisms of these waters in the subarctic North Pacific and their importance in creating deep ocean stratification with potential impacts on ocean carbon storage. We also address several modeling caveats in representing only surface sea ice in the present generation of climate models (not allowing for subsurface freezing) and in ensuring tracer conversation in longterm transient climate model simulations.

 

How to cite: Ishizu, M., Timmermann, A., and Kyung-Sook, Y.: A brief note on Supercooled Glacial Deep Waters, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14091, https://doi.org/10.5194/egusphere-egu25-14091, 2025.

EGU25-14317 | ECS | Orals | CL4.11

New Insolation Forcing for Paleoclimate Models 

Ilja J. Kocken and Richard E. Zeebe

In paleoclimate simulations, the insolation forcing at the top of the atmosphere needs to be altered to reflect Earth's orbital history during the time interval of interest. General Circulation Models (GCMs) often rely on either a modern orbital configuration to allow for direct comparison to modern and near-future climate simulations—sometimes with snapshot sensitivity experiments (DeepMIP, PlioMIP, etc.)—or they use the Berger (1978) (Ber78) routines to compute the orbital parameters. For snapshot simulations targeting older time periods such as the Eocene, using the modern orbital configuration is inappropriate, because the obliquity amplitude, for example, was much smaller than in the recent past. Our astronomical solutions ZB18a and ZB20a have been shown to produce the best match with geologic data to 58 Ma and 71 Ma, respectively (Zeebe & Lourens 2019, Kocken & Zeebe 2024). The eccentricity of the Ber78 solution diverges from these astronomical solutions already at ~33 ka, shows a different amplitude throughout, and drifts out of phase at ~1.6 Ma. It has been noted in the literature as well as code that the Ber78 routines are not appropriate for an analysis of time periods older than ~1 Myr. However, even recent transient simulations of the past 3 Myr sometimes fall back to using these outdated routines for the full time period. This is likely because of their ease of use; for example, the Ber78 routines are well-integrated into the Community Earth System Model (CESM).

In this study, we analyze the effects of using recent astronomical solutions on the insolation at the top of the atmosphere. Here we show that the absolute difference between insolation from Ber78 and our solution ZB18a increases periodically with increasing age, reaching values up to 88 Wm−2 at 2.68 Ma. This difference is of the same order of magnitude as the difference between a precession minimum and maximum. To facilitate using recent astronomical solutions in GCMs such as the CESM, we make the ZB18a and ZB20a orbital solutions readily available: We provide Fortran subroutines that calculate insolation and interpolate the astronomical parameters to a certain calendar date, and provide drop-in replacements to existing Fortran subroutines from the CESM. In this presentation we will show several examples of previous studies that could have benefited from these new routines.

Berger, A. (1978). Long-term variations of caloric insolation resulting from the earth’s orbital elements, Quaternary Research, 9, 139–167. https://doi.org/10.1016/0033-5894(78)90064-9

Zeebe, R. E., & Lourens, L. J. (2019). Solar System chaos and the Paleocene–Eocene boundary age constrained by geology and astronomy. Science, 365(6456), 926–929. https://doi.org/10.1126/science.aax0612

Kocken, I.J., & Zeebe, R. E. (2024). Testing Astronomical Solutions With Geological Data for the Latest Cretaceous: An Astronomically Tuned Time Scale. Paleoceanography and Paleoclimatology, 39(11). https://doi.org/10.1029/2024PA004954

How to cite: Kocken, I. J. and Zeebe, R. E.: New Insolation Forcing for Paleoclimate Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14317, https://doi.org/10.5194/egusphere-egu25-14317, 2025.

EGU25-14580 | ECS | Orals | CL4.11

Remote impacts of the mid-Holocene Green Sahara 

Shivangi Tiwari, Francesco S. R. Pausata, Allegra N. LeGrande, Michael Griffiths, Ilana Wainer, Hugo Beltrami, Anne de Vernal, Peter O. Hopcroft, Clay Tabor, Deepak Chandan, and W. Richard Peltier

The mid-Holocene (MH: 6,000 years before present) is a key time slice for paleoclimate studies, and is one of the two entry cards for participation in the current Paleoclimate Modelling Intercomparison Project (PMIP4). The MH was characterized by high boreal summer insolation, leading to an intensification of the Northern Hemisphere monsoons. In northern Africa, the strengthening of the West African Monsoon was further amplified by nonlinear feedbacks, resulting in the development of vegetation referred to as the “Green Sahara”. The vegetation and land surface changes over northern Africa had various remote effects impacting the global climate through teleconnections.

In this study, we analyse outputs from five fully coupled global climate models to identify the  remote impacts of the Green Sahara on global climate. Through the difference of two sets of mid-Holocene simulations – with and without the Green Sahara – we isolate the effect of the northern African vegetation and land cover changes on South American hydroclimate and tropical modes of climate variability such as the El Niño Southern Oscillation and the Atlantic Niño. Using an atmosphere-only climate model, we further investigate the Saharan-Arctic teleconnection invoked to explain the Arctic cooling concurrent with Saharan desertification. We quantify proxy-model agreement through metrics such as the Cohen’s Kappa index and the Root Mean Square Error to assess if the inclusion of the Green Saharan changes leads to greater coherence of model simulations with proxy reconstructions. Our results demonstrate the critical role of the Green Sahara in modulating the MH climate.

How to cite: Tiwari, S., S. R. Pausata, F., N. LeGrande, A., Griffiths, M., Wainer, I., Beltrami, H., de Vernal, A., O. Hopcroft, P., Tabor, C., Chandan, D., and Peltier, W. R.: Remote impacts of the mid-Holocene Green Sahara, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14580, https://doi.org/10.5194/egusphere-egu25-14580, 2025.

EGU25-15686 | Posters on site | CL4.11

Estimating the change in low level cloud cover during the Brunhes-Matuyama magnetic field reversal: A first modelling approach 

Irina Thaler, Jacob Svensmark, Martin Bødker Enghoff, Nir Shaviv, and Henrik Svensmark

Geomagnetic variations are the perfect testbed to study the effect of Galactic Cosmic Rays (GCR) on climate, as they disentangle solar variability from direct GCR effects. We use the 3D chemical transport model GEOS-CHEM to simulate the change in the cloud condensation nuclei number density during the Brunhes-Matuyama magnetic field reversal assuming present day aerosol conditions. We then estimate the change in cloud condensation nuclei for low level clouds under both solar minimum and solar maximum ionisation conditions. We also test whether the effect of ion-enhanced growth significantly enhances the process. We find a cloud condensation nuclei enhancement for low level clouds throughout the magnetic field reversal of several percent, which supports the observational findings of a wetter and colder climate during the Brunhes-Matuyama magnetic field reversal.

How to cite: Thaler, I., Svensmark, J., Bødker Enghoff, M., Shaviv, N., and Svensmark, H.: Estimating the change in low level cloud cover during the Brunhes-Matuyama magnetic field reversal: A first modelling approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15686, https://doi.org/10.5194/egusphere-egu25-15686, 2025.

EGU25-17020 | ECS | Posters on site | CL4.11

Antarctic ice sheet evolution from the Last Glacial Maximum to the present day constrained by relative sea-level variations 

Jonas Van Breedam, Philippe Huybrechts, and Elie Verleyen

The Last Glacial Maximum (LGM) Antarctic ice sheet extent is relatively well constrained with an ice sheet reaching to the continental shelf edge in most places. The ice mass stored in the ice sheet and especially the ice sheet mass loss evolution since the Last Glacial Maximum is more debated. Reconstructed relative sea-level (RSL) variations along the Antarctic coast capture the interplay between ice mass changes, variations in the isostatic response and gravitational forces between the ocean water and the ice mass and therefore, can aid to reconstruct the Antarctic ice sheet evolution from the LGM to the present day.

Here we use the Antarctic ice sheet model AISMPALEO that includes a spatially variable Elastic Lithosphere Relaxing Asthenosphere isostasy model with an approximation of the gravitational consistent sea level equation. A large suite of Antarctic ice sheet model simulations is performed and analyzed from the Last Glacial Maximum to the present-day. The simulations are forced by different global sea-level reconstructions, PMIP4 climate model output for the ocean and the atmosphere and different Earth rheological parameters in the isostasy model. The model runs are compared with published datasets of relative sea-level along the coast of Antarctica to derive the best agreement between the RSL data and the Antarctic ice sheet evolution.

How to cite: Van Breedam, J., Huybrechts, P., and Verleyen, E.: Antarctic ice sheet evolution from the Last Glacial Maximum to the present day constrained by relative sea-level variations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17020, https://doi.org/10.5194/egusphere-egu25-17020, 2025.

EGU25-17858 | Orals | CL4.11

Simulating marine biogeochemistry and atmospheric pCO2 for the Last Glacial Maximum using an ensemble of calibrated parameter sets 

Chia-Te Chien, Markus Pahlow, Markus Schartau, Christopher Somes, and Andreas Oschlies

During the Last Glacial Maximum (LGM), atmospheric pCO2 was approximately 90 ppm lower than in the pre-industrial era. Several hypotheses have been proposed to explain this decrease, including changes in nutrient supply, increased iron input to the ocean, and variations in overturning circulation strength driven by differences in wind stress and moisture diffusivity. Current modeling approaches that simulate LGM marine biogeochemistry typically use parameter sets calibrated under pre-industrial boundary conditions, introducing uncertainty due to the imperfect knowledge of the values that can be assigned to the parameters for the LGM environment. The extent to which this uncertainty affects the simulated LGM marine biogeochemistry remains unclear. In this study, we employ an optimality-based non-Redfield plankton ecosystem model coupled with a 3D Earth system model to simulate LGM conditions. We conduct sensitivity analyses with 24 combinations of biogeochemical parameters (reduced benthic denitrification rate, decreased sedimentary iron input, higher PO4 levels, and increased atmospheric iron depositio­n) and physical boundary conditions (changes in wind stress pattern and increased meridional moisture diffusivity over the Southern Ocean). For each scenario, we perform 20 simulations using 20 biogeochemical parameter sets selected out of 600—each representing pre-industrial biogeochemistry and evaluated based on the misfit between observations and model outputs—resulting in a total of 480 simulations. Our results show that iron input exerts the most profound influence on LGM marine biogeochemistry and atmospheric pCO2, while changes in major nutrient supplies have minor effects. Additionally, the impact of physical conditions on biogeochemical tracers varies, depending on the specific biogeochemical settings. Compared to pre-industrial reference conditions, atmospheric pCO2 under full LGM conditions decreases by 36 to 58 ppm across the 20 simulations. The difference between the maximum and minimum pCO2 changes amounts to 50% of the 43 ppm average decrease. These findings highlight that, although the 20 parameter sets effectively reproduce pre-industrial marine biogeochemistry, significant cross-model variance in pCO2 responses and marine biogeochemical changes persists under LGM conditions.

How to cite: Chien, C.-T., Pahlow, M., Schartau, M., Somes, C., and Oschlies, A.: Simulating marine biogeochemistry and atmospheric pCO2 for the Last Glacial Maximum using an ensemble of calibrated parameter sets, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17858, https://doi.org/10.5194/egusphere-egu25-17858, 2025.

EGU25-17910 | Posters on site | CL4.11

Planning for the next phase of the Paleoclimate Modelling Intercomparison Project (PMIP7) 

Chris Brierley, Masa Kageyama, Jean-Yves Peterschmitt, Christian Stepanek, and Louise Sime

The Paleoclimate Modelling Intercomparison Project (PMIP) was launched in 1995 and has since closely followed the phases of the Coupled Model Intercomparison Project (CMIP) providing understanding of past climate states based on the latest Global Climate Models and evaluation of their capacity to represent climates very different from the recent one. PMIP is planning its next phase, in the wake of CMIP7 launch (Dunne et al., 2024).

CMIP7 is organised along two main phases: the Fast Track, to be delivered in time for its results to be analysed and published for the seventh assessment report of the IPCC (Intergovermental Panel on Climate Change), followed by the main phase of CMIP7. This poster will describe the rationale of including an idealised paleoclimate simulation, "abrupt-127k", in the Fast Track set of experiments. This experiment starts from the Fast Track pre-industrial control experiment and then abruptly changes the astronomical parameters to those for 127,000 years ago (as well as some minor greenhouse gas changes). This will allow analyses of the sensitivity of the Arctic sea ice to conditions favouring its summer decrease or even collapse, and can be extended to become a last interglacial simulation (lig127k). The poster will also briefly describe the other experiments that are expected to be included in the next phase of PMIP. We are looking forward to discussions of key experiments, analyses, challenges with the PMIP and CMIP communities alike.

Dunne et al., 2024: https://doi.org/10.5194/egusphere-2024-3874

How to cite: Brierley, C., Kageyama, M., Peterschmitt, J.-Y., Stepanek, C., and Sime, L.: Planning for the next phase of the Paleoclimate Modelling Intercomparison Project (PMIP7), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17910, https://doi.org/10.5194/egusphere-egu25-17910, 2025.

EGU25-18286 | ECS | Posters on site | CL4.11

Ice-sheet topography changes in North America affect teleconnection patterns on glacial time scales 

Isma Abdelkader Di Carlo, Francesco Pausata, Masa Kageyama, Cécile Davrinche, Marcus Lofverstrom, and Ulysses Ninnemann

The topography of the Laurentide Ice Sheet (LIS) during glacial periods, particularly the Last Glacial Maximum (LGM), played a pivotal role in shaping atmospheric circulation and teleconnection patterns. This study investigates the impact of LIS elevation changes on global atmospheric dynamics using fully coupled paleoclimate simulations with the isotope-enabled Community Earth System Model (CESM) version 1.2. Previous studies have shown that a higher LIS elevation significantly amplifies Arctic warming, reducing the equator-to-pole temperature gradient and influencing jet streams and stationary waves (Liakka & Lofverstrom, 2018 ; Beghin et al., 2014 ; Lofverstrom et al., 2014). This mechanism may also extend to the Southern Hemisphere, affecting teleconnection pathways.

By systematically modifying LIS elevation, we explore its role in altering large-scale atmospheric circulation features such as the Intertropical Convergence Zone (ITCZ), Southern Annular Mode (SAM), and Walker circulation, as well as modes of variability including El Niño–Southern Oscillation (ENSO). We show the critical influence of LIS topography on global teleconnections and how ice sheet dynamics shaped glacial climate variability and atmospheric feedbacks.

How to cite: Abdelkader Di Carlo, I., Pausata, F., Kageyama, M., Davrinche, C., Lofverstrom, M., and Ninnemann, U.: Ice-sheet topography changes in North America affect teleconnection patterns on glacial time scales, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18286, https://doi.org/10.5194/egusphere-egu25-18286, 2025.

EGU25-18941 | ECS | Posters on site | CL4.11

Enhanced “wind-evaporation effect” drove the “deep-tropical contraction” in the early Eocene 

Zikun Ren, Tianjun Zhou, Zhun Guo, Meng Zuo, Lingqiang He, Xiaolong Chen, Lixia Zhang, Bo Wu, and Wenmin Man

The early Eocene is the warmest epoch in the last 65 million years, with a global mean temperature 9 to 23°C higher than the modern era. According to state-of-the-art climate models, the tropical rainfall contracted towards the equator during this extremely warm period. However, the physical mechanism causing this phenomenon remains unclear. In this study, we examined the hemispheric energy balance in the early Eocene that causes the equatorward contraction of tropical precipitation. A novel mechanism underlying this phenomenon is revealed. Based on the climate modeling of CESM1.2, we show that the GHG-induced warmth enhances the sensitivity of evaporation to surface wind speed changes in the early Eocene. Thus, the stronger tropical trade wind in the winter hemisphere will drive out stronger latent heat flux than in the summer hemisphere. This interhemispheric asymmetric response reduces the interhemispheric heating contrast in the solstice seasons. As a result, the ascending motion in the tropical atmosphere migrates towards the equator, finally decreases the width of tropical precipitation in the early Eocene.

How to cite: Ren, Z., Zhou, T., Guo, Z., Zuo, M., He, L., Chen, X., Zhang, L., Wu, B., and Man, W.: Enhanced “wind-evaporation effect” drove the “deep-tropical contraction” in the early Eocene, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18941, https://doi.org/10.5194/egusphere-egu25-18941, 2025.

EGU25-19034 | Posters on site | CL4.11

Monsoon trend and multi-scale variability changes over the last 6000 years 

Roberta D'Agostino, Pascale Braconnot, Sandy P. Harrison, Julien Crètat, Zhenqian Wang, and Qiong Zhang and the PACMEDY

The Holocene started about 10000 years before present and is the period during civilizations as we know them today emerged. However, during that time several regions such as Sahel-Sahara or the Indus valley in the tropics experienced severe aridification and dramatic environmental changes for ecosystems and humans. There is general agreement that this has been caused by the southward shift of the boreal monsoon rain belt and that slow variations of Earth’s orbital parameters are the long-term driver. In addition to insolation forcing, several feedbacks involving the ocean, sea-ice, or vegetation have had a profound impact on regional changes and on the multiscale monsoon variability, including extreme monsoon years. They have shaped the magnitude and the timing of environmental changes depending on monsoon systems. Although these feedbacks have been widely discussed, their relative strength is still under debate. These unknows prevent proper anticipation and simulation of future monsoon behavior. Long transient simulations of the Holocene climate allow us to revisit these questions by shedding light on monsoon multiscale variability and the representation of vegetation feedbacks. Using a set of transient mid to late Holocene simulations (last 6000 years), we will discuss the relative evolution of the global monsoons. Highlights will be on the relative responses to changes in insolation seasonality between African and Indian monsoons, the role of dynamical versus thermodynamical atmospheric feedbacks in monsoon precipitation, and on the relationship between long term trends, interannual to multicentennial variability and periods of extreme dry or wet monsoon seasons. Comparisons of model results with proxy reconstruction of climate variability over land and ocean from speleothems, coral and shells has been done considering the chaotic nature of multiscale monsoon variability. They provide us with indication of the consistency of model inferred trends in monsoon variability and the real climate trajectory.

How to cite: D'Agostino, R., Braconnot, P., Harrison, S. P., Crètat, J., Wang, Z., and Zhang, Q. and the PACMEDY: Monsoon trend and multi-scale variability changes over the last 6000 years, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19034, https://doi.org/10.5194/egusphere-egu25-19034, 2025.

EGU25-20327 | Posters on site | CL4.11

Insights from AWIESM-wiso:  climate and water isotope signals in northern Africa in a precession cycle 

Xiaoxu Shi, Martin Werner, Hu Yang, Qinggang Gao, Jiping Liu, and Gerrit Lohmann

Precessional forcing is a key driver of quaternary climate change. Based on 24 experiments covering a full precession cycle, this study explores spatio-temporal variations of both climate and isotope signals in northern Africa. We find a synchronous phasing of precipitation variations with solar radiation levels and an asynchronous timing of surface air temperature changes across different sub-regions of northern Africa. Based on daily precipitation, our results reveal earlier onset and withdrawal, as well as a shorter duration of the West Africa summer monsoon (WASM) at minimum precession compared to maximum precession. The onset of the WASM is controlled by the intensity of the Sahara Heat Low, while the monsoon termination is linked to subtropical solar radiation and interhemispheric thermo contrast. Using a novel scale-flux tracing technique, we find that, precipitation during minimum precession is more influenced by evaporation from warmer and more humid regions compared to maximum precession. Additionally, certain inland areas of northern Africa exhibit positive temporal isotope-precipitation gradients, violating the "amount effect". This phenomenon mainly occurs during precession phases associated with Green Sahara periods. The isotope composition changes in such places primarily reflect changes in upstream rainfall quantity, rather than changes in local precipitation as is inferred from present day analogs. Conversely, the "amount effect" remains applicable during dry periods in Africa when the Sahara desert is present. This suggests that isotope-based reconstruction of past precipitation variations during Green Sahara periods over North Africa needs to be taken with caution.

How to cite: Shi, X., Werner, M., Yang, H., Gao, Q., Liu, J., and Lohmann, G.: Insights from AWIESM-wiso:  climate and water isotope signals in northern Africa in a precession cycle, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20327, https://doi.org/10.5194/egusphere-egu25-20327, 2025.

NP6 – Turbulence, Transport and Diffusion

EGU25-473 | ECS | Orals | NP6.1

Turbulent Lagrangian fCO2 time series statistics in the Southern Ocean 

Kévin Robache and François G. Schmitt

The Southern Ocean plays a crucial role in regulating Earth's climate, absorbing approximately 10 % of annual human CO2 emissions (DeVries, 2014; Friedlingstein et al., 2023). However, it is still a challenge to fully understand its carbon dynamics due to significant observational gaps, particularly during winter. Furthermore, the dynamics on small spatial and temporal scales are also poorly understood, despite their potential importance in shaping the overall carbon budget of the region (Guo & Timmermans, 2024). Between 2001 and 2012, researchers from the LOCEAN laboratory in Paris deployed 15 CARIOCA Lagrangian drifting buoys in this region to gain a deeper understanding of its spatial carbon dynamics (Boutin et al., 2008; Resplandy et al., 2014) at high-frequency (1-hour time resolution). In this study, we analyzed the time series of six of these buoys in the framework of Lagrangian turbulence (Kolmogorov, 1941; Landau & Lifschitz, 1944; Inoue, 1951). This is done using Lagrangian data on CO2 fugacity (fCO2), chlorophyll a, sea surface temperature (SST), and sea surface salinity (SSS) along their trajectories. Additionally, we examined the dynamics of the buoys' drifting speeds estimated from buoys location data.

Through Fourier spectral analysis and structure function analysis, we demonstrated that these time series exhibit scaling and intermittent behaviour, in agreement with the Lagrangian vision of the turbulent Richardson-Kolmogorov energy cascade in fully developed turbulence. Notably, at least two distinct spectral regimes were identified. Chlorophyll a and fCO2 behave as active turbulent scalars, while SST and SSS depicted statistics compatible with passive scalars with a higher intermittency on timescales shorter than 4 days. The links between these time series were also investigated, using the generalized correlation functions (GCFs) and exponents (GCEs).

References :

DeVries, T. (2014). The oceanic anthropogenic CO2 sink: Storage, air‐sea fluxes, and transports over the industrial era. Global Biogeochemical Cycles28(7), 631-647.

Friedlingstein, P. et al. (2023). Global carbon budget 2023. Earth System Science Data, 15(12), 5301-5369.

Guo, Y., & Timmermans, M. L. (2024). The role of ocean mesoscale variability in air‐sea CO2 exchange: A global perspective. Geophysical Research Letters51(10), e2024GL108373.

Boutin, J. et al. (2008). Air‐sea CO2 flux variability in frontal regions of the Southern Ocean from CARbon Interface OCean Atmosphere drifters. Limnology and Oceanography53(5part2), 2062-2079.

Resplandy, L. et al. (2014). Observed small spatial scale and seasonal variability of the CO2 system in the Southern Ocean. Biogeosciences11(1), 75-90.

Kolmogorov, A. N. (1941). On degeneration (decay) of isotropic turbulence in an incompressible viscous liquid. In Dokl. Akad. Nauk SSSR (Vol. 31, pp. 538-540).

Landau L.D. & Lifshitz E.M. (1944). Fluid Mechanics (MIR), first russian edition.

Inoue, E. (1952). Turbulent fluctuations in temperature in the atmosphere and oceans. Journal of the Meteorological Society of Japan. Ser. II30(9), 289-295.

How to cite: Robache, K. and Schmitt, F. G.: Turbulent Lagrangian fCO2 time series statistics in the Southern Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-473, https://doi.org/10.5194/egusphere-egu25-473, 2025.

EGU25-1290 | Posters on site | NP6.1

Dispersal of invasive species larvae within the Orust-Tjörn fjord system 

Sandra-Esther Brunnabend, Lars Arneborg, and Sam Fredriksson

The Orust-Tjörn fjord system is located on the west coast of Sweden and consists of several fjords connected by shallow and narrow straits. It is home to nature reserves, harbors, leisure areas, and aquaculture farms, and biodiversity is threatened by invasive species, for example brought in through shipping. Therefore, it is important to understand how larvae of invasive species are dispersed by the currents within the fjords system in order to find efficient methods for management of existing and future harmful invasive species. 

A connectivity study is performed in order to identify dispersion patterns, assuming that larvae are passively transported by surface currents. For the years 2016 and 2022, the dispersion of larvae is simulated using the open source Opendrift software (Dagestad et al., 2018). The model is forced by velocity fields modeled with a high resolution regional Nemo3.6 ocean model with lateral resolution of ~50m. A large number of particles (~700,000) are seeded with four-day intervals, covering the whole fjord system and areas of open waters near the entrances of the fjord system. For each seeding, the dispersion model runs for 3 weeks where larvae that reach a shore are transported away again when currents change (pelagic phase). This is followed by a one-week period where larvae settled as soon as they reach a shore (settling phase). On the basis of this ensemble, we perform a connectivity analysis indicating the probabilities of larvae, released at one location, settling in other locations within the fjord system.

Results show that larvae seeded inside the Orust-Tjörn fjord system mostly remain there with some even remaining in the same local fjord basin during the four-week period. Connectivity matrices also show that some larvae travel far. Larvae seeded outside the Orust-Tjörn fjord system are likely to leave the model domain as they are transported within the generally northward flowing swift Baltic current. 

How to cite: Brunnabend, S.-E., Arneborg, L., and Fredriksson, S.: Dispersal of invasive species larvae within the Orust-Tjörn fjord system, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1290, https://doi.org/10.5194/egusphere-egu25-1290, 2025.

EGU25-1454 | ECS | Posters on site | NP6.1

An Adaptive Masking Time Series Transformer based Representation Learning Model for Well Log Curves 

Pin Li, Jun Zhou, Yubo Liu, Juan Zhang, Guojun Li, and Yuange Zhou

Well log curves, acquired from downhole logging tools during well logging, are pivotal for reservoir characterization and formation evaluation in oil and gas exploration and production. However, manual feature extraction from raw curves remains essential for constructing effective machine learning models, presenting time-consuming challenges and stringent labeling requirements. Concurrently, the transformer architecture, prevalent in NLP and computer vision, offers promise for representation learning. This paper proposes a self-supervised transformer based methodology for extracting well log curves representations, aiming to expedite downstream model development.

While transformer models have gained prominence in handling text and image data, well log curves present a distinct challenge as they resemble time series data. Despite the nascent development of time series transformer models, we conducted an extensive review of current progress and adopted the best-performing time series transformer model for extracting representations from well log curves. Importantly, given the challenges posed by factors such as borehole conditions and instrument failure, certain types of well log curves may occasionally be missing or distorted. To address this issue, our proposed methodology introduces an adaptive masking mechanism, which selectively applies masking to patches of curves where data quality is poor, thereby effectively mitigating data quality concerns.

Data from 2000 wells are utilized for model training, with an additional 100 wells reserved for validation purposes. Our study observed a consistent decrease in both training and test losses until convergence during the training stage. Initially, mean squared error (MSE) and mean absolute error (MAE) are employed to quantify reconstruction errors between reconstructed curves and raw curves, low values of MSE (0.08) and MAE (0.07) indicate effectiveness of the learned representations. Subsequently, a downstream task involving oil and gas identification is undertaken, wherein a classification model is developed based on representations learned by the transformer model. Performance comparison between models utilizing learned representation and those employing statistical features highlights the superior performance of the former (98% accuracy), emphasizing the efficacy of our representation learning methodology. This paper introduces a novel self-supervised methodology based on transformer architecture for well log curve representation learning. The method automates information extraction without requiring logging expertise and substantially enhances downstream machine learning model performance.

How to cite: Li, P., Zhou, J., Liu, Y., Zhang, J., Li, G., and Zhou, Y.: An Adaptive Masking Time Series Transformer based Representation Learning Model for Well Log Curves, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1454, https://doi.org/10.5194/egusphere-egu25-1454, 2025.

EGU25-3171 | ECS | Orals | NP6.1

Lagrangian tracking of particles settling through the atmosphere: influence of particle shape on its dispersion 

Taraprasad Bhowmick, Florencia Falkinhoff, Eberhard Bodenschatz, and Gholamhossein Bagheri
All solid particles in the atmosphere – such as ash, dust, ice crystals, pollen and microplastics – are non-spherical, which affects their atmospheric transport. However, studies of their dispersion are often based on models derived from measurements in stationary fluids or on field data distorted by atmospheric fluctuations. To address these limitations, the IMPACT (In-situ Measurement of Particles, Atmosphere, Cloud, and Turbulence) field campaign was conducted in northern Finland during May and June 2024. As part of this initiative, we launched an innovative experiment to track the dispersion of small, non-spherical particles released at altitudes between 2 and 7 km. Their trajectories were monitored until they reached the ground.
 
The experiment used particles of consistent mass (8.5 grams) and volume but varying shapes, including icosahedrons (representing near-spherical forms), as well as circular and elliptical discs, some with perforations. Up to 20 paperboard particles equipped with miniaturized, battery-powered electronics were placed inside a biodegradable helium balloon for each launch. At the target altitude, the balloon burst, releasing the particles from a single point. Throughout the particles' ascent within the balloon and their descent after release, GPS data on their position and altitude were transmitted via radio to ground stations. Over the course of the campaign, we tracked up to 150 particles across six distinct shapes. In addition, particle-resolved direct numerical simulations are carried out to determine the settling behavior in still air as a function of particle shape. In this presentation, we will share preliminary findings on particle dispersion patterns and explore the influence of atmospheric turbulence on the behavior of non-spherical particles.

How to cite: Bhowmick, T., Falkinhoff, F., Bodenschatz, E., and Bagheri, G.: Lagrangian tracking of particles settling through the atmosphere: influence of particle shape on its dispersion, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3171, https://doi.org/10.5194/egusphere-egu25-3171, 2025.

EGU25-4715 | Orals | NP6.1

Nonlinear causal dependencies as a signature of the complexity of the climate dynamics 

Stéphane Vannitsem, X. San Liang, and Carlos A. Pires

Nonlinear quadratic and linear dynamical dependencies of large-scale climate modes are disentangled through the analysis of the rate of the information transfer. That is performed in a joint analysis of eight dominant climate modes, covering the tropics and extratropics over the North Pacific and Atlantic. A clear signature of nonlinear and compound influences at low-frequencies (time scales larger than a year) are emerging, while high-frequencies are only affected by linear dependencies. These results point to the complex nonlinear collective behavior at global scale of the climate system at low-frequencies, supporting earlier views that regional climate modes are local expressions of a global intricate low-frequency variability dynamics, which is still to be fully uncovered.

How to cite: Vannitsem, S., Liang, X. S., and Pires, C. A.: Nonlinear causal dependencies as a signature of the complexity of the climate dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4715, https://doi.org/10.5194/egusphere-egu25-4715, 2025.

EGU25-5726 | ECS | Posters on site | NP6.1

Manifold Embeddings for Multispectral Time-Series Land Disturbance Detection 

Mengyao Li and Jianbo Qi

Dimensionality reduction techniques have been successfully applied in remote sensing to reduce redundant information. However, achieving dimensionality reduction and lossless recovery for multispectral data at any global location remains a challenge, particularly given the complex and variable nature of surface conditions. Furthermore, it is still unclear if the reduced features maintain temporal continuity and can be effectively integrated with existing time series algorithms for disturbance detection. This study trains a Uniform Manifold Approximation and Projection (UMAP) model based on Harmonized Landsat Sentinel-2 (HLS) imagery to accomplish multispectral dimensionality reduction. Subsequently, the manifold embeddings are used in the Continuous Change Detection and Classification (CCDC) algorithm for land disturbance detection. Two key conclusions are drawn from this study: 1) a general multispectral dimensionality reduction model was constructed based on UMAP, which is applicable to all global land surfaces and any seasons. The manifold embeddings exhibit a stable value range and preserve the coherence of the time series. 2) compared to full-spectrum multispectral data, the manifold embeddings achieved comparable performance in image prediction and disturbance detection. Our study demonstrates the potential of manifold learning-based representation of global land surface reflectance spectra for lightweight storage and processing of dense satellite image time series, while keeping the ability to detect any kinds of land disturbance.

How to cite: Li, M. and Qi, J.: Manifold Embeddings for Multispectral Time-Series Land Disturbance Detection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5726, https://doi.org/10.5194/egusphere-egu25-5726, 2025.

EGU25-5876 | Orals | NP6.1

Relative dispersion at the surface of the ocean: role of balanced motions and internal waves 

Stefano Berti, Michael Maalouly, Guillaume Lapeyre, and Aurélien Ponte

Ocean flows at scales smaller than few hundreds of kilometers display rich dynamics, mainly associated with quasi- geostrophic motions and internal gravity waves. Although both of these processes act on comparable lengthscales, the former, which include meso and submesoscale turbulent flows, are considerably slower than the latter, which take part in the ocean fast variability. Understanding how their effects overlap is crucial for several fundamental and applied questions, including the interpretation and exploitation of new, high-resolution satellite altimetry data, and the characterization of material transport at fine scales.

In this study we investigate these points by examining Lagrangian pair-dispersion statistics in a high-resolution global-ocean numerical simulation including high-frequency motions, such as internal gravity waves. In particular, we aim at assessing the sensitivity of the particle relative-dispersion process on ageostrophic, fast fluid motions. For this purpose we select a study area close to Kuroshio Extension, characterized by energetic submesoscales, and focus on the seasonal variability of the Lagrangian dynamics.

We find that in winter pair dispersion is predominantly influenced by meso and submesoscale motions, meaning nearly balanced dynamics. The behavior of the different Lagrangian indicators considered agrees in this case with the theoretical predictions, based on the shape of the kinetic energy spectrum, in quasi-geostrophic turbulent flows. Conversely, in summer, when high-frequency motions gain importance and submesoscales are less energetic, the situation is found to be more subtle, and the usual relations between dispersion properties and spectra do not seem to hold. We explain this apparent inconsistency relying on a decomposition of the flow into nearly-balanced motions and internal gravity waves. Through this approach, we show that while the latter contribute to the kinetic energy spectrum at small scales, they do not impact relative dispersion, which is essentially controlled by the nearly-balanced, mainly rotational, flow component at larger scales.

How to cite: Berti, S., Maalouly, M., Lapeyre, G., and Ponte, A.: Relative dispersion at the surface of the ocean: role of balanced motions and internal waves, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5876, https://doi.org/10.5194/egusphere-egu25-5876, 2025.

EGU25-6863 | ECS | Posters on site | NP6.1

Spatiotemporal Causal Effect Estimation in Complex Dynamical Systems 

Rebecca Herman and Jakob Runge

Causal Inference is essential for identifying and quantifying causal relationships in systems where randomized controlled experiments are infeasible, but the high dimensionality and co-variability structure of spatiotemporal dynamical systems such as the climate system pose special challenges for causal effect estimation. It is standard for climate scientists to reduce the dimension of their data with pre-processing procedures such as regional means and principal component analysis, but taking a regional mean may mask differences in spatial pattern – such as the difference between Eastern Pacific and Central Pacific El Niño events – that may be relevant for causal relationships. Similarly, principal component analysis may obscure true causal relationships because the spatial pattern associated with maximum co-variability may not be the causally relevant information. Instead of using these preprocessing techniques, the basic procedure of time series causal effect estimation can be simply extended to multivariate time series, but this introduces new complications and heightens already existing complications of time series causal effect estimation. Here, we discuss these complications and present practical solutions. Complications for multi-variate as well as univariate time series include: (1) neighboring points in time and space may be very similar if the scale of the spatiotemporal sampling rate is small relative to the characteristic scale of the variance, resulting in unstable estimations, (2) the do-calculus expression for estimating the response to a hard intervention may include calculations with spatiotemporal gradients so strong they would result in instabilities in the system, and finally, (3) it is often not possible to actually perform a hard intervention in dynamical systems, making the interpretation of the causal effect unclear. The first complication may be addressed using L2 regularization, and the second and third complications may be addressed by focusing on soft interventions of reasonable magnitude that approach zero on their spatiotemporal boundaries. A unique complication of multi-variate causal effect estimation is that, when using L2 regularization, the total causal influence of a climate variable will be penalized inverse-proportionally to the number of spatial datapoints. This complication can be addressed by scaling variables so that the total spatiotemporal variance, rather than the component-wise variance, is one. We showcase the power of the technique by quantifying the spatiotemporal causal effect of El Niño-related sea surface temperature variability on atmospheric pressure variability in the North Atlantic in unforced Community Earth System Model simulations. We demonstrate that spatiotemporal causal effect estimation allows us to simultaneously determine the relevant spatial patterns and more accurately quantify a pattern-dependent causal effect between ENSO and NAO that has thus far proven difficult to measure in observational studies.

How to cite: Herman, R. and Runge, J.: Spatiotemporal Causal Effect Estimation in Complex Dynamical Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6863, https://doi.org/10.5194/egusphere-egu25-6863, 2025.

EGU25-6918 | ECS | Orals | NP6.1

New ABL measurements of Lagrangian relative dispersion by means of radiosonde clusters 

Niccolo' Gallino, Shahbozbek Abdunabiev, John Craske, Ben Devenish, Jennyfer Tse, and Daniela Tordella

Turbulent relative dispersion is a phenomenon of fundamental interest both for its theoretical implications and for its immediate applications, which in geophysical sciences range from pollutant spreading in the atmosphere to nutrient transport in the oceans. We present new results in the measurement of turbulent relative dispersion in the atmospheric boundary layer, which enrich the picture with respect to the current framework. The measurements were carried out using clusters of miniaturized radiosondes, carried by small (~40 cm in diameter) helium balloons [1]. These clusters enable the effective investigation of relative dispersion by computing inter-particle distances among radiosondes. This methodology represents a concrete attempt at realising the type of analysis originally conceived by L. F. Richardson in his 1926 paper [2], often regarded as the one that initiated the field of study of relative dispersion.

The current accepted framework for the discussion of relative dispersion is the Kolmogorov-Obukhov scaling theory, which on dimensional grounds allowed for the derivation of the result (called the Richardson-Obukhov law) according to which the mean square distance in between particles advected by a turbulent flow field scales like the cube of time, , where ε is the energy dissipation rate and g is called the Richardson constant. However, this result is only valid for the case of homogeneous, isotropic turbulence, specifically in the inertial range of scales [2, 3]. Atmospheric turbulence, instead, is far from homogeneity and isotropy, and is characterized by local intense intermittency and entrainment [4, 5].
We conducted six cluster launches across three distinct topographical environments: the near-maritime plains at Chilbolton Observatory, the western Alps near the Astronomical Observatory of Aosta Valley, and the hilly region surrounding Udine. The results reveal not only deviations from the RO law but also significant variations between launches and distinct dispersion regimes within each launch (Fig. 1). The implication is, as expected, that the dispersion law for the atmosphere does not have a universal character, and depends on specific details of the boundary layer flow. The next step in the analysis will be the identification of the relevant flow features which impact the dispersion law, which is especially challenging due to the wide range of possibly participating phenomena.


Fig. 1. Mean square separation distance between mini-radiosondes within the cluster during six field experiment flights in different environmental topologies. Cross symbols show results from the MET OFFICE NAME dispersion model [6].

1. Abdunabiev S. et al., Measurement 224, 113879 (2024)
2. Richardson LF, Proc. R. Soc. Lond. A 110, 709 (1926)
3. Devenish, BJ, Thomson DJ. JFM 867, 877–905 (2019)
4. Van Reeuwijk M, Vassilicos JC, Craske J. JFM 908 (2021)
5. Fossa’ L., Abdunabiev S., Golshan M., Tordella D., Physics of fluids 34, (2022)
6. Turbulence_&_Diffusion_Note_288, Met Office, UK (2003)

How to cite: Gallino, N., Abdunabiev, S., Craske, J., Devenish, B., Tse, J., and Tordella, D.: New ABL measurements of Lagrangian relative dispersion by means of radiosonde clusters, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6918, https://doi.org/10.5194/egusphere-egu25-6918, 2025.

In past decades, increasing robust causal models were proposed, making causal inference under different scenarios and data limitations feasible. On one hand, these causal model are all based on time series data sources. On the other hand, in Earth Science, some variables, such as soil features and elevation, do not present a time series or the time series of these variables do not present sufficient temporal variations. In this case, traditional temporal causal models may fail to identify these clearly existing causalities in Earth Science.  To fill these gaps, here we show a Geographical Convergent Cross Mapping (GCCM) model for spatial causal inference with spatial cross-sectional data based cross-mapping prediction in reconstructed state space. Three typical cases, where clearly existing causations cannot be measured through temporal models, demonstrate that GCCM could detect weak-moderate causations when the correlation is not significant. And when the coupling between two variables is significant and strong, GCCM is advantageous in identifying the primary causation direction and better revealing the bidirectional asymmetric causation, overcoming the mirroring effect. The principle and some cases of GCCM are briefly introduced.  

How to cite: Chen, Z.: Causal Inference in GeoScience: From the Temporal to Spatial Dimensions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7326, https://doi.org/10.5194/egusphere-egu25-7326, 2025.

EGU25-11012 | Posters on site | NP6.1

Enhanced Ocean Model Predictability through Integration of High-Frequency Radar Observations and 2DVAR Data Assimilation: A Case Study of Pasaia Port 

Guillermo García Sánchez, Irene Ruiz, Anna Rubio, and Lohitzune Solabarrieta

Accurate ocean state forecasting is fundamental for effective port operations and coastal zone management. In the southeastern Bay of Biscay, particularly Pasaia port, high-resolution ocean condition forecasts directly impact navigation safety, port logistics, and environmental monitoring capabilities. The integration of observational data with numerical models represents a critical advancement in improving forecast accuracy for operational oceanography applications.

This study addresses the challenge of enhancing ocean model performance through a systematic approach to data assimilation. We focus on incorporating high-frequency (HF) radar observations into the Iberian-Biscay-Irish (IBI) regional model framework to optimize boundary conditions of the MOHID model that is available in the area. The motivation stems from the need to reduce forecast uncertainties in coastal areas where complex bathymetry, tidal forcing, and meteorological conditions interact. By implementing a two-dimensional variational (2DVAR) assimilation scheme, we aim to minimize the discrepancies between model outputs and observational data, ultimately providing more reliable ocean state estimates for local maritime operations. To validate the improved model outputs, we will compare them against Lagrangian drifter trajectories using a skill score metric, ensuring the assimilation’s effectiveness in capturing complex ocean dynamics.

How to cite: García Sánchez, G., Ruiz, I., Rubio, A., and Solabarrieta, L.: Enhanced Ocean Model Predictability through Integration of High-Frequency Radar Observations and 2DVAR Data Assimilation: A Case Study of Pasaia Port, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11012, https://doi.org/10.5194/egusphere-egu25-11012, 2025.

EGU25-11509 | ECS | Orals | NP6.1

Sparse pre-whitening operators for regression of climatic time series 

Donald P. Cummins and Mengheng Li
Regression methods are used extensively in climate science and are commonly applied to output from numerical climate models, e.g. for detection and attribution of climate change trends and for diagnosing emergent properties of climate models such as Equilibrium Climate Sensitivity (ECS). Output from climate models can have complex spatiotemporal dependence structures and, in practice, the assumptions of the Gauss-Markov Theorem seldom hold. Under such conditions, the application of Ordinary Least Squares (OLS) is inefficient and can lead to biased inference, with implications for model selection and evaluation.

The detection and attribution community has traditionally addressed this problem using a Generalised Least Squares (GLS) approach, whereby a pre-whitening operator is estimated from a climate model's pre-industrial control (piControl) simulation, typically using an unstructured sample covariance matrix or regularised version thereof.

We show how, for low-dimensional collections of climate variables, the dependence structure can be parsimoniously parameterised as a Vector AutoRegression (VAR) and the resultant sparse pre-whitening operator efficiently computed. For the first-order VAR(1) model, this procedure is analogous to a multivariate Prais-Winsten estimation. An example application to calibration of Simple Climate Models (SCMs) is discussed, shedding new light on the problem of choosing an appropriate model complexity.

How to cite: Cummins, D. P. and Li, M.: Sparse pre-whitening operators for regression of climatic time series, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11509, https://doi.org/10.5194/egusphere-egu25-11509, 2025.

EGU25-11547 | ECS | Posters on site | NP6.1

Vortex dynamics on Rotating Penetrative Convection 

Gabriel Meletti, Thierry Alboussière, Jezabel Curbelo, Stéphane Labrosse, and Philippe Odier

This work presents experimental results regarding rotating penetrative convection. The focus is on how convection driven by thermal or salty composition interacts with a stably stratified region. In such systems, as convection overshoots into the stratified layer, complex feedback loops arise, leading to the generation of internal waves that propagate in the stably stratified region. In rotating systems, Coriolis effects can further modify the dynamics, giving rise to inertial-gravity waves in the stably stratified region. Furthermore, the convective cells can change into different patterns of elongated vortices, changing how convection overshoots, and how it can drive internal waves. These phenomena are relevant to different geophysical and astrophysical applications, such as in the Earth's atmosphere, where internal gravity waves are excited in the stratosphere by convective motions in the troposphere. These interactions are also relevant to planetary and stellar interior applications, where convection can drive waves in stably stratified layers such as the radiative zone of stars or in the (possibly existing) stratified layer at the Earth's external core, where rotation effects are even more significant due to the small Rossby numbers, of the order of $10^{-5}$ to $10^{-4}$. This indicates that rotational forces dominate over inertial forces, highlighting the importance of better understanding the effects of rotation in the dynamics of penetrative convection and wave interactions.

Our experimental setup, named \textit{CROISSANTS (Convective ROtational Interactions with Stable Stratification Arising Naturally in Thermal Systems)}, found at the Physics Laboratory of the Ecole Normale Supérieure (ENS) de Lyon, is mounted on a rotating table and investigates the dynamics of rotating systems using water with a temperature gradient. The temperature ranges from approximately $30^oC$ at the top of a $30$cm-high cubic cavity and decreases to $0^oC$ at the bottom. Since water exhibits a density inversion between $0^oC$ and $4^oC$, the system naturally develops convection at the bottom, beneath a stably stratified region that extends from the convective interface to the top of the cavity. Measurements were performed using techniques such as Particle Image Velocimetry (PIV), Schlieren techniques, and Laser-Induced Fluorescence (LIF), to capture the convective and wave motions in both vertical and horizontal planes. Numerical simulations complement the experiments, exhibiting similar behavior to the observed experimental results. Both experiments and numerical simulations show that the elongated vortices in the convective region can be observed in higher regions of the stable density stratified zone. These long-lasting vortices move slowly in the flow (compared to the rotation of the experiment). Lagrangian-Averaged-Vorticity-Deviation (LAVD) techniques are then applied to track the dynamics of these long-lasting vortices elongated in the stable region. Understanding these processes provides a framework for interpreting how convective motion transfers energy across scales, impacting large-scale magnetic fields and planetary evolution.

How to cite: Meletti, G., Alboussière, T., Curbelo, J., Labrosse, S., and Odier, P.: Vortex dynamics on Rotating Penetrative Convection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11547, https://doi.org/10.5194/egusphere-egu25-11547, 2025.

Natural magnetic field measurement is essential for discovering fundamental physical mechanisms in space. Both the CSES mission and the DEMETER satellite equipped with the search coil magnetometer to observe the magnetic field waves. The CSES mission’s search coil magnetometer was developed by the School of Space Sciences Department of Beihang University. But the accuracy of these measurements is often degraded by artificial interference from reaction wheels on satellites. These wheels produce complex harmonic interference, often overlapping with the natural signal in both time and frequency domain, which makes it difficult to observe natural signals.

Traditional methods usually construct filters to separate interference. Advanced signal technologies have focused on reducing interference using self-adaptive signal decomposition methods in either time or frequency domain. In this field, Finley and Robert have used singular spectrum analysis to remove interference from in situ magnetic field data from the CASSIOPE/Swarm-Echo mission. But they did not settle the time-frequency overlap problem. In fact, most signal decomposition methods do not work well. These methods usually damage the natural signal because the overlapping areas remain indistinguishable.

In this paper, a novel method named the Instantaneous Phase Discontinuity (IPD) method is proposed to address this issue. Based on the sensitivity of instantaneous phase to variation of signal frequency, this method utilizes the discontinuities in the phase function to identify overlapping time-frequency regions. Subsequently, the natural signal within the overlapping region is carefully separated through frequency band contraction and envelope correction. IPD holds broad application prospects. As an example, IPD effectively separates interference from the time-frequency overlapping regions while preserving the integrity of natural signals when applied to data obtained from the CSES mission.

How to cite: Shi, F., Zeng, L., and Fu, Y.: An Innovative Technique for Reaction wheel Interference Separation in Satellite Magnetic Field Signals, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11558, https://doi.org/10.5194/egusphere-egu25-11558, 2025.

EGU25-11897 | Posters on site | NP6.1

Numerical studies of connectivity and Lagrangian transport in the world’s oceans 

Viacheslav Kruglov and Ulrike Feudel

Particles transport can be used to study flow fields on different scales in geophysics. Tracer and inertial particle transport can highlight the connectivity between different locations in the ocean or describe changes in flow fields based on the visualization of the flow by tracers. Of particular interest are long-range transport properties to either identify changes in flow paths due to climate change or to study the transport of seeds over long distances to identify sources of plants in different parts of the world. Such studies require particle tracking algorithms which are capable to work properly on a global scale of the Earth, i.e. on a spherical geometry. 

We have created a sophisticated software tool that simulates the movement of large numbers of tracer and inertial particles within interpolated oceanic velocity fields, in our examples based on the publicly available HYCOM data. Built in C++ and parallelized with Intel Threading Building Blocks (Intel TBB), it achieves high performance when dealing with substantial computational loads. To accelerate nearest-neighbor searches, we organize the grid points into a kd-tree, making it quick to locate grid points near any particle. We then interpolate the eastward and northward velocity components using a Gaussian-shaped weight function — an effective choice that avoids the singularities sometimes encountered in inverse distance interpolation. Since planar projections can introduce significant distortions on a global scale, we also account for Earth’s spherical geometry. Specifically, we solve two-dimensional tracer equations and the Maxey–Riley equation for inertial particles on a local tangent plane. Afterward, we revert the computed particle positions to latitude-longitude coordinates via an azimuthal equidistant projection, mitigating large-scale errors in simulations that may span thousands of kilometers.

The software is capable of simulating the dispersal of seeds and algae by ocean currents, easily managing hundreds of thousands of particles under varied initial conditions. It reconstructs connectivity maps between distant coasts, identifies transport barriers through finite-time Lyapunov exponent calculations, and can compute derivatives of the velocity field — such as divergence, vorticity, and the Okubo–Weiss parameter — broadening its range of oceanographic applications.

We highlight the software’s capabilities with two representative examples. First, we track the origins of particles (such as plant seeds) and explore their possible routes to Hawaii. Second, we assess the likelihood that harmful algal blooms could drift into the Baffin Bay during the warmest parts of the summer.

How to cite: Kruglov, V. and Feudel, U.: Numerical studies of connectivity and Lagrangian transport in the world’s oceans, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11897, https://doi.org/10.5194/egusphere-egu25-11897, 2025.

EGU25-13384 | Orals | NP6.1

Confinement and shedding 

Bernard Legras, Aurélien Podglajen, Mariem Rezig, and Clair Duchamp

Large-scale atmospheric vortices like the polar vortex or the Asian monsoon anticyclone are known to confine compounds for several months in the corresponding regions of the stratosphere with many consequences on the transport and the resulting atmospheric composition, the chemical activity and radiative properties.

It was recently discovered that confinement over the same time scale occurs also in much smaller mesoscale anticyclonic vortices generated within the absorbing plumes of smoke or ash generated by large forest fires and some volcanic eruptions.

As a rule, the atmosphere dissipates rapidly all inertial structures and these vortices are all maintained by a sustained forcing. We will discuss the similarities and differences among those vortices, the smoke vortices being distinguished by their autonomy as they carry their own source of forcing when they travel around the globe.

We will discuss the phenomenon of isentropic vortex shedding which is a main mechanical dissipation factor and show that it behaves very similarly at all scales. In the vertical direction, the flux processor of the large vortices will be compared to and distinguished from the leaking process of the rising smoke vortices. Other processes associated with radiative relaxation of thermal anomalies play role both to maintain and dissipate.

Although the state of understanding of smoke vortices is still very incomplete, a discussion of their condition of formation, maintenance and stability will be offered based on observations and idealized numerical simulation.

How to cite: Legras, B., Podglajen, A., Rezig, M., and Duchamp, C.: Confinement and shedding, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13384, https://doi.org/10.5194/egusphere-egu25-13384, 2025.

EGU25-14793 | ECS | Orals | NP6.1

On uniting Eulerian and Lagrangian mesoscale eddy perspectives 

Stella Bērziņa, Aaron Wienkers, Nicolas Gruber, and Matthias Münnich

Mesoscale eddies play a pivotal role in oceanic dynamics, influencing transport, mixing, and energy distribution. Current detection methods are primarily divided into Eulerian and Lagrangian approaches, each highlighting unique eddy characteristics. Eulerian methods rely on instantaneous fields, such as sea surface height, Okubo–Weiss parameter or vorticity, to identify the eddy boundaries. In contrast, Lagrangian approaches utilize water parcel trajectories to compute metrics like the Lagrangian Average Vorticity Deviation (LAVD) or Finite-Time Lyapunov Exponents (FTLE), identifying rotationally coherent Lagrangian vortices (RCLVs) with minimal exchange across the boundary. Eulerian eddies, however, are inherently "leaky", allowing for fluid exchange due to the fact that their boundaries are non-material. Despite these differences, both approaches capture complementary aspects of the same physical phenomenon. This study aims to bridge the gap between the two eddy detection methods by combining their strengths and leveraging high-resolution simulations from the coupled climate model ICON. Here, we identify daily RCLVs from evolving LAVD fields to find the time at which each Eulerian eddy loses coherence. In doing so, we will be able to explore how eddy coherence changes though its lifecycle and geographical location. This combined methodology can deepen our understanding of mesoscale ocean transport by quantifying realistic eddy trapping ability.

How to cite: Bērziņa, S., Wienkers, A., Gruber, N., and Münnich, M.: On uniting Eulerian and Lagrangian mesoscale eddy perspectives, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14793, https://doi.org/10.5194/egusphere-egu25-14793, 2025.

EGU25-17867 | ECS | Posters on site | NP6.1

An Intensive Biomass Burning Aerosol Observation phase in 2022, over Skukuza, South Africa: CO transport and balance over Southern Africa 

Marion Ranaivombola, Nelson Bègue, Gisèle Krysztofiak, Lucas Vaz Peres, Venkataraman Sivakumar, Gwenaël Berthet, Fabrice Jegou, Stuart Piketh, and Hassan Bencherif

The Biomass Burning Aerosol Campaign (BiBAC) was conducted in the Kruger National Park (KNP), at Skukuza in South Africa during the 2022 biomass burning season. The campaign included an Intensive Observation Phase (IOP) from September to October, aiming to quantify aerosol optical properties and plume transport.(Ranaivombola et al., 2024). The combination of ground-based (sun-photometer), satellite observations (MODIS, IASI and CALIOP), and CAMS reanalysis show a significant aerosol and carbon monoxide (CO) loading linked to biomass burning activity. Using AOD data from sun-photometer observations, Ranaivombola et al., (2024) define two events of biomass burning plume over the Southwestern Indian Ocean (SWIO) basin: September 18 to 23 and October 9 to 17, called here after event 1 and event 2, respectively.

During Event 1, the plume was transported toward the SWIO basin as a "river of smoke" phenomenon. As reported previously in the literature (Swap et al., 2003 and Flamant et al., 2022), the meteorological conditions were influenced by the passage of westerly waves associated with a cut-off low (COL) that favored the eastern transport pathway. However, it was not the case during Event 1. There were two troughs which supported the formation of two frontal systems and contributed to the transport of aerosols and CO plumes from South America (SAm) towards Southern Africa (SA). This transport was driven by a westerly baroclinic wave through the mid-tropospheric layers.

Event 2 involved a more complex synoptic setup with three frontal systems supported by three distinct troughs, allowing the recirculation of plumes over SA. This dynamic system enhanced the transport of CO plumes from SAm, which merged with African plumes over the Mozambique Channel. The sustained activity of the baroclinic wave generated new troughs, keeping aerosol levels high for an extended period of 1.5 week. The progression of baroclinic waves and frontal system development were essential in driving regional and intercontinental transport of aerosols and CO plumes.

These two events allowed to reveal two transport mechanisms of aerosol plumes and CO between SAm and SA towards the SWIO basin. It shows also that SA is a target region for aerosols and CO from SAm biomass burning. To assess and quantify the contributions of SA and SAm sources to observed CO concentrations over SA, we used the FLEXPART model (version 10.4) coupled with CO emissions database (biomass burning and anthropogenic emission from CAMS: GFAS and CAMS-GLOB-ANT, respectively). Each simulation tracked particles representing CO back in time over a period of 20 days, during the IOP. The setup included daily releases of 20,000 particles over six sites in Southern Africa (Skukuza, Durban, Maun, Upington, Mongu and Gobabeb). Both SA and SAm sources significantly influenced the CO balance over SA. The contribution of biomass burning emissions from SA were higher than those from SAm. Nevertheless, the biomass burning emission from SAm were more variable and could occasionally match or exceed those from SA. This quantification confirmed the predominance of African sources but also highlighted the presence of intercontinental transport which is poorly investigated until now.

How to cite: Ranaivombola, M., Bègue, N., Krysztofiak, G., Vaz Peres, L., Sivakumar, V., Berthet, G., Jegou, F., Piketh, S., and Bencherif, H.: An Intensive Biomass Burning Aerosol Observation phase in 2022, over Skukuza, South Africa: CO transport and balance over Southern Africa, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17867, https://doi.org/10.5194/egusphere-egu25-17867, 2025.

EGU25-19212 | Posters on site | NP6.1

A Lagrangian Estimate of the Mediterranean Outflow's Origin 

Giulia Vecchioni, Paola Cessi, Nadia Pinardi, Louise Rousselet, and Francesco Trotta

The Mediterranean Sea is characterized by an anti-estuarine circulation, with Atlantic Water entering the Strait of Gibraltar at the surface and denser waters, formed within the basin, exiting at depth as the Mediterranean Outflow. Early studies identified the Western Mediterranean Deep Water, formed in the Gulf of Lions, as the primary source of the dense water masses contributing to the Outflow. While confirming this finding, more recent analyses of in-situ observations have highlighted additional contributions from other intermediate and deep water masses, such as Western Intermediate Water, Levantine Intermediate Water and Tyrrhenian Deep and Intermediate Waters.

In this study, the origin of the Mediterranean Outflow is investigated by deploying six million Lagrangian parcels at the Strait of Gibraltar, and advecting them backward in time using velocity estimates from an eddy-permitting reanalysis. Trajectories are integrated until parcels reach one of three origin sections within a maximum time of 78 years. To estimate the transport exchange between the origin sections and the Strait of Gibraltar, each parcel is tagged with a small volume transport, which is conserved along the trajectories due to the non-divergence of the velocity field.

The results indicate that 86% of the Outflow's transport originates from the Gulf of Lions, associated with Western Mediterranean Deep Water and Western Intermediate Water; 13% from the Strait of Sicily, related to Levantine Intermediate Water; and 1% from the Northern Tyrrhenian, related to Tyrrhenian Deep and Intermediate Waters. Mediterranean dense waters all recirculate in the Algerian Basin and in the deep Tyrrhenian basin, where stirring and mixing processes are hypothesized to occur. Before exiting the Strait of Gibraltar, anticyclonic recirculation induced by the western Alboran gyre decreases the density and depth of the water mass, ultimately shaping the characteristics of the Mediterranean Outflow. Temperature-salinity histograms at each origin section exhibit broad distribution, with peaks corresponding to expected water-mass types. The median transit times from the sections to the Strait of Gibraltar range from 5 years (Gulf of Lions) to 8 years (Strait of Sicily).

How to cite: Vecchioni, G., Cessi, P., Pinardi, N., Rousselet, L., and Trotta, F.: A Lagrangian Estimate of the Mediterranean Outflow's Origin, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19212, https://doi.org/10.5194/egusphere-egu25-19212, 2025.

This study investigates the 3-D Lagrangian evolution of Madagascar cyclonic eddies and their interaction with the Agulhas Current, combining targeted Argo float experiments, satellite altimetry data, and ocean modeling, following three in situ experiments. The region of interest spans from southwest Madagascar, where the South East Madagascar Current detaches from the continental shelf and generates dipoles, to the KwaZulu-Natal Bight, where the Agulhas Current flows southward.

The first two experiments, conducted in April and July 2013, deployed eight Argo floats configured to measure temperature and salinity at high temporal resolutions (daily and five-daily) and at varying park depths (300, 500, 650, and 1,000 m). These deployments assessed float retention within two cyclonic eddies that propagated southwestward over 130 days at an average speed of 11 km/day, undergoing growth, maturity, and decay phases before interacting with the Agulhas Current. A third experiment, conducted from May to September 2022, deployed two Euro-Argo ERIC-managed Core Argo floats southwest of Madagascar to further explore eddy dynamics. These floats drifted at non-standard depths of 650 m and 800 m, with adaptive cycle intervals (daily, 2-daily, and 5-daily) based on the eddy's proximity to the Agulhas Current. This experiment also captured the eastward propagation of the cyclonic eddy and its interaction with the current. In all three experiments, the floats exited the eddy when positioned below the depth at which the eddy's nonlinearity ratio dropped below 1. Complementary numerical simulations used an eddy identification and tracking algorithm with the GLORYS12V1 reanalysis product. Virtual particle releases and Lagrangian tracking at depths matching the above Argo float parking levels replicated the field experiments. Numerical results aligned with observations, showing that cyclonic eddies exhibited greater trapping depths during their mature phase and shallower depths during the growth and decay phases.

By integrating targeted float experiments, satellite data, and numerical simulations, this study provides a comprehensive understanding of eddy trapping dynamics southwest of Madagascar and their role in transporting heat, salt, and biogeochemical properties into the Agulhas Current. These findings demonstrate the potential of GLORYS12V1 combined with numerical Lagrangian particle tracking to address observational gaps in traditionally undersampled regions and underscore the benefits of combining ad hoc Argo configurations and numerical simulations for studying 3-D eddy dynamics.

How to cite: Aguiar González, B. and Morris, T.: Assessing the Trapping Dynamics of Madagascar Cyclonic Eddies Through Non-Standard Argo Float Experiments and Numerical Lagrangian Particle Tracking, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19267, https://doi.org/10.5194/egusphere-egu25-19267, 2025.

EGU25-437 | ECS | Orals | NP6.2

Pattern Formation of Rotating Magnetoconvection with Anisotropic Thermal Diffusivity Effect in the Earth's Outer Core 

Krishnendu Nayak, Hari Ponnamma Rani, Jaya Krishna Devanuri, Yadagiri Rameshwar, and Jozef Brestenský

The rotation rate and the magnetic field play a key role, in the geodynamo models, for understanding the convective flow behavior in the Earth’s outer core where dynamic MAC balance of forces occurs frequently and is affected by the diffusion processes. Due to the presence of buoyancy, Lorentz and Coriolis forces, the turbulent eddies in the core get deformed and elongated in the direction parallel to the rotation axis and magnetic field in BM anisotropy or are affected by gravity (buoyancy) direction in SA anisotropy. Hence the turbulence is highly anisotropic. The turbulent small-scale eddies are diffusers of momentum and heat, and thus, the effective viscosity and thermal diffusion are also anisotropic. The effect of anisotropic thermal diffusion coefficient on the stability of horizontal fluid planer layer heated from below and cooled from above, rotating about its vertical axis and subjected to a uniform horizontal magnetic field, is analyzed in the present study. The cross, oblique and parallel rolls assumed to make an angle (θ), 90°, 0° < θ < 90° and 0°, respectively, with the axis of the magnetic field. These rolls are calculated for different range of control parameters arising in the system. The linear stability analysis is investigated by using the normal mode method. The appearance of rolls for stationary modes as well as oscillatory modes depends on the SA (Stratification Anisotropy) parameter, α (the ratio of horizontal and vertical thermal diffusivities). The stabilizing/destabilizing effect strongly depends on the Chandrasekar (Q) and Taylor (Ta) numbers. The obtained results for isotropic cases coincide with those obtained by pioneers in the literature. The two-dimensional anisotropic complex Ginzburg-Landau (ACGL) equation with cubic nonlinearity is used to study the weakly nonlinear behaviour near the primary instability threshold. This equation, derived using the multiple scale analysis, is similar to the one found in the literature. The numerical simulation of this ACGL equation with periodic boundary conditions has been carried out using the pseudo-spectral method in Fourier space with exponential time differencing. The formation of spatiotemporal patterns strongly depends on α, Ta and Q. For fixed Q, as Ta increases, the Coriolis force intensifies, more stable and organized spiral patterns showed their presence. Further for increasing Ta, the size or scale of spiral patterns decreases, while the number of patterns get increased. 

How to cite: Nayak, K., Rani, H. P., Devanuri, J. K., Rameshwar, Y., and Brestenský, J.: Pattern Formation of Rotating Magnetoconvection with Anisotropic Thermal Diffusivity Effect in the Earth's Outer Core, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-437, https://doi.org/10.5194/egusphere-egu25-437, 2025.

EGU25-2092 | ECS | Posters on site | NP6.2

Stratification governs the Existence of Surface-Intensified Eastward Jets in Turbulent Ocean Gyres 

Lennard Miller, Bruno Deremble, and Antoine Venaille

We investigate the impact of stratification on the formation and persistence of turbulent eastward jets in the ocean (like the Gulf Stream and Kuroshio extensions) [1]. Using a wind-driven, two-layer quasi-geostrophic model in a double-gyre configuration, we construct a phase diagram to classify flow regimes. The parameter space is defined by a criticality parameter ξ, which controls the emergence of baroclinic instability, and the ratio of layer depths δ, which describes the surface intensification of stratification. Eastward jets detaching from the western boundary are observed when δ < 1 and ξ ~ 1, representing a regime transition from a vortex-dominated western boundary current [2] to a zonostrophic regime characterized by multiple eastward jets. The emergence of the coherent eastward jet is further addressed with complementary 1.5-layer simulations and explained through both linear stability analysis and turbulence phenomenology. In particular, we show that coherent eastward jets emerge when the western boundary layer is stable, and find that the asymmetry in the baroclinic instability of eastward and westward flows plays a central role in the persistence of eastward jets,while contributing to the disintegration of westward jets.

[1] Miller, L., Deremble, B., & Venaille, A. (2024). Stratification governs the Existence of Surface-Intensified Eastward Jets in Turbulent Gyres without Bottom Friction. ( https://arxiv.org/abs/2411.05660 )

[2] Miller, L., Deremble, B., & Venaille, A. (2024). Gyre turbulence: Anomalous dissipation in a two-dimensional ocean model. Physical Review Fluids9(5), L051801.

How to cite: Miller, L., Deremble, B., and Venaille, A.: Stratification governs the Existence of Surface-Intensified Eastward Jets in Turbulent Ocean Gyres, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2092, https://doi.org/10.5194/egusphere-egu25-2092, 2025.

EGU25-2737 | ECS | Posters on site | NP6.2

Existence of Bolgiano–Obukhov scaling in the bottom ocean? 

Peng-Qi Huang, Shuang-Xi Guo, Sheng-Qi Zhou, Xian-Rong Cen, Ling Qu, Ming-Quan Zhu, and Yuan-Zheng Lu

Boundary layer dynamics is key to understanding energy and mass transport in the bottom ocean. Due to observational limitations, the structure of bottom water and its scaling behavior have been relatively under-researched. The seminal Bolgiano–Obukhov (BO) theory established the fundamental framework for turbulent mixing and energy transfer in stably stratified fluids. However, the presence of BO scalings remains debatable despite their being observed in stably stratified atmospheric layers and convective turbulence. In this study, we performed precise temperature measurements with 51 high-resolution loggers above the seafloor for 46 h on the continental shelf of the northern South China Sea (116°E,21.2°N,278 m). The temperature observation exhibits three layers with increasing distance from the seafloor: the bottom mixed layer (BML), the mixing zone and the internal wave zone. A BO-like scaling α = −1.34 ± 0.10 is observed in the temperature spectrum when the BML is in a weakly stable stratified and strongly sheared  condition, whereas in the unstably stratified convective turbulence of the BML, the scaling α = −1.76 ± 0.10 clearly deviated from the BO theory but approached the classical −5/3 scaling in isotropic turbulence. This suggests that the convective turbulence is not the promise of BO scaling. In the mixing zone, where internal waves alternately interact with the BML, the scaling follows the Kolmogorov scaling. In the internal wave zone, the scaling α = −2.12 ± 0.15 is observed in the turbulence range and possible mechanisms are provided.

How to cite: Huang, P.-Q., Guo, S.-X., Zhou, S.-Q., Cen, X.-R., Qu, L., Zhu, M.-Q., and Lu, Y.-Z.: Existence of Bolgiano–Obukhov scaling in the bottom ocean?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2737, https://doi.org/10.5194/egusphere-egu25-2737, 2025.

EGU25-3191 | Orals | NP6.2

Hydraulic control, turbulence and mixing in stratified buoyancy-driven exchange flows 

Paul Linden, Amir Atoufi, Adrien Lefauve, and Lu Zhu

Buoyancy-driven exchange flows in geophysical contexts, such as flows through straits, often create a partially-mixed intermediate layer through mixing between the two stratified counterflowing turbulent layers. We present a three-layer hydraulic analysis of such flows, highlighting the dynamical importance of the intermediate layer. Our model is based on the viscous, shallow water, Boussinesq equations and includes the effects of mixing as a non-hydrostatic pressure forcing. We apply this shallow-water formulation to direct numerical simulations of stratified inclined duct (SID) exchange flows where turbulence is controlled by a modest slope of the duct. We show that the nonlinear characteristics of the three-layer model correspond to linear long waves perturbing the three-layer mean flow, and predict, in agreement with recent experimental observations in SID, hydraulically-controlled regions in the middle of the duct, linked to the onset of instability and turbulence. We also provide the first evidence of long-wave resonance, as well as resonance between long and short waves, and their connection to transitions from intermittent to fully developed turbulence. These results challenge current parameterisations for turbulent transport in stratified exchange flows, which typically overlook long waves and internal hydraulics induced by streamwise variations of the flow.

How to cite: Linden, P., Atoufi, A., Lefauve, A., and Zhu, L.: Hydraulic control, turbulence and mixing in stratified buoyancy-driven exchange flows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3191, https://doi.org/10.5194/egusphere-egu25-3191, 2025.

EGU25-3703 | ECS | Posters on site | NP6.2

A model for small-scale ocean turbulence based on wave turbulence theory 

Nicolas Lanchon and Pierre-Philippe Cortet

It has long been proposed that small-scale oceanic dynamics results from nonlinear processes involving internal gravity waves. The scales in question are not resolved in oceanic models but are accounted for by ad-hoc parameterizations. Physically modelling their turbulent dynamics would therefore be a lever for improving parameterizations in climate models.

In this context, a promising avenue is the weakly nonlinear wave turbulence theory. Its implementation in the case of internal waves in density stratified fluids has nevertheless proved complex and remains an open problem. It is the subject of delicate questions concerning the convergence of the so-called “collision integral” which drives the dynamics in wave turbulence problems.

In this talk, we examine the weak turbulence theory in a linearly stratified fluid from a new perspective. We derive a simplified version of the kinetic equation of internal gravity wave turbulence. The keystone is the assumption that the energy transfers are dominated by a class of nonlocal resonant interactions, known as the “induced diffusion” triads, which conserve the ratio between the wave frequency and the vertical wave number. This kinetic equation allows us to derive scaling laws for the spatial and temporal energy spectra which are consistent with typical exponents observed in the oceans. Our analysis also remarkably shows that the internal wave turbulence cascade is associated to an apparent constant flux of wave action.

How to cite: Lanchon, N. and Cortet, P.-P.: A model for small-scale ocean turbulence based on wave turbulence theory, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3703, https://doi.org/10.5194/egusphere-egu25-3703, 2025.

EGU25-4591 | ECS | Orals | NP6.2

Wave-Turbulence Cascades and Deep Ocean Mixing: Inferring Diapycnal Diffusivity in High-Resolution Ocean Models 

Kayhan Momeni, William R. Peltier, Joseph Skitka, Yuchen Ma, Brian K. Arbic, Yulin Pan, and Dimitris Menemenlis

Internal wave dynamics play a critical role in understanding ocean diapycnal diffusivity and associated mixing processes, particularly in the deep ocean context. Building upon prior analyses of internal wave breaking and its influence on diapycnal diffusivity, in this study we employ a high-resolution regional ocean model to infer ocean diapycnal diffusivity due to internal wave (IW) breaking [Momeni et al., 2025]. Our work leverages the Bouffard-Boegman parameterization, which distinguishes between reversible and irreversible mixing components. This framework provides a robust methodology to infer diapycnal diffusivity profiles from turbulent dissipation rates, improving upon earlier KPP-based approaches that lacked this critical distinction. This inference is made possible through the work of Skitka et al. [2024], which directly measured dissipation rates from numerical simulations.

The findings reinforce and expand on earlier results from dynamically downscaled simulations in the northeast Pacific, which revealed a pronounced wave-turbulence cascade and highlighted the suppression of higher-order IW modes due to the background component of KPP. By deactivating this component, higher-order modes engage in triad resonance interactions with lower-order modes and are effectively energized; they subsequently undergo shear instability, enhancing mixing rates and aligning diffusivity profiles with empirical observations. This mechanism is discussed in detail in Momeni et al. [2024].

Our results underscore KPP’s limitations in distinguishing mixing processes and its tendency to overestimate shear contributions to diffusivity. These insights pave the way for improving diapycnal diffusivity parameterizations in low-resolution climate models by emphasizing mechanisms rooted in internal wave breaking rather than simplified parameterizations. Future work will focus on higher-resolution simulations to refine these findings and address basin- and latitude-dependent variations.

 

References

Kayhan Momeni, Yuchen Ma, William R Peltier, Dimitris Menemenlis, Ritabrata Thakur, Yulin Pan, Brian K Arbic, Joseph Skitka, and Matthew H Alford. Breaking internal waves and ocean diapycnal diffusivity in a high-resolution regional ocean model: Evidence of a wave-turbulence cascade. Journal of Geophysical Research: Oceans, 129(6):e2023JC020509, 2024.

Kayhan Momeni, W Richard Peltier, Joseph Skitka, Yuchen Ma, Brian K Arbic, Dimitris Menemenlis, and Yulin Pan. An alternative buoyancy reynolds number-based inference of ocean diapycnal diffusivity due to internal wave breaking: results from a high-resolution regional ocean model. Geophysical Research Letters, 2025. Submitted for publication.

Joseph Skitka, Brian K Arbic, Yuchen Ma, Kayhan Momeni, Yulin Pan, William R Peltier, Dimitris Menemenlis, and Ritabrata Thakur. Internal-wave dissipation mechanisms and vertical structure in a high-resolution regional ocean model. Geophysical Research Letters, 51(17):e2023GL108039, 2024.

How to cite: Momeni, K., Peltier, W. R., Skitka, J., Ma, Y., Arbic, B. K., Pan, Y., and Menemenlis, D.: Wave-Turbulence Cascades and Deep Ocean Mixing: Inferring Diapycnal Diffusivity in High-Resolution Ocean Models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4591, https://doi.org/10.5194/egusphere-egu25-4591, 2025.

EGU25-5953 | ECS | Orals | NP6.2

The influence of oceanic bottom slopes on eddy mixing in a two-layer model 

Miriam Sterl, André Palóczy, Joe LaCasce, Sjoerd Groeskamp, and Michiel Baatsen

Oceanic mesoscale eddy mixing plays a crucial role in the Earth’s climate system by redistributing heat, salt and carbon. Eddy mixing is impacted by various physical factors, one of which is the oceanic bottom slope. Within a barotropic framework, it can be shown analytically that bottom slopes suppress the cross-slope eddy mixing. Unfortunately, adding baroclinic effects greatly increases the complexity of the problem. To understand how bottom slopes influence eddy mixing in a baroclinic framework, we study eddy fields in a quasi-geostrophic two-layer model with a linear bottom slope. We investigate the eddy mixing by releasing and tracking virtual particles in the flow fields and analysing how they spread in the cross-slope direction. This is done for a range of bottom slope magnitudes and for prograde as well as retrograde slopes. The goal is to figure out how eddy mixing depends on the steepness and direction of the bottom slope and on the position in the water column. We find that for steep bottom slopes, the baroclinic instability is suppressed, the eddy field gets weaker, and the spreading of particles in the cross-slope direction decreases. This suppression is comparable for prograde and retrograde slopes. Moreover, the suppression is observed not only in the bottom layer, where the slope is located, but also in the upper layer. This indicates that the suppression of eddy mixing by oceanic bottom slopes can have an impact throughout the water column.

How to cite: Sterl, M., Palóczy, A., LaCasce, J., Groeskamp, S., and Baatsen, M.: The influence of oceanic bottom slopes on eddy mixing in a two-layer model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5953, https://doi.org/10.5194/egusphere-egu25-5953, 2025.

EGU25-6814 | ECS | Orals | NP6.2

Analysis of Mesoscale Dynamics in the Mesosphere using Radar Observations and Machine Learning 

Vincent Joel Peterhans, Juan Miguel Urco, Victor Avsarkisov, and Jorge L. Chau

One of the main factors characterizing the dynamics of the atmosphere is its vertical density stratification. Gravity waves arising under these conditions play an essential role in large-scale energy transport through upwards propagation and breaking in the middle atmosphere, manifesting in phenomena such as the cold summer mesopause. Moreover, it was recently found that the summer mesopause is also home to the strongly stratified turbulence regime occurring at extremely high buoyancy Reynolds and low horizontal Froude numbers. Direct observation or numerical simulation of these processes with high resolution proves difficult however, due to the remoteness of the region combined with the mesoscale horizontal and small vertical scales that have to be resolved for a detailed analysis of the emerging dynamics. 

To deepen our knowledge of the these processes in this region, we employ a combined approach of state-of-the-art radar observations using the MAARSY and SIMONe systems and the physics-informed machine learning method HYPER. The first step and the main topic of the current study is to reconstruct high-resolution 3D wind fields from the line-of-sight measurements in the summer mesosphere. The resulting fields closely capture the observed data and produce high-fidelity, Navier-Stokes-compliant predictions of the surrounding flow beyond measuring points. Building on this, we aim to provide an analysis of the first high-resolution radar observations of strongly stratified turbulence in the middle atmosphere.

How to cite: Peterhans, V. J., Urco, J. M., Avsarkisov, V., and Chau, J. L.: Analysis of Mesoscale Dynamics in the Mesosphere using Radar Observations and Machine Learning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6814, https://doi.org/10.5194/egusphere-egu25-6814, 2025.

EGU25-7085 | ECS | Posters on site | NP6.2

Rotating Stratified Turbulence 

Dante Buhl, Pascale Garaud, and Hongyun Wang

Recent interest in the dynamics of stratified turbulence has led to the development of new models for quantifying vertical transport of momentum and buoyancy (Chini et al. 2022, Shah et al. 2024). These models are still incomplete as they do not yet include all of the relevant dynamics often present in real physical settings such as rotation and magnetic fields. Here we expand on prior work by adding rotation. We conduct 3D direct numerical simulations of rotating, stochastically forced, strongly stratified turbulence (Fr << 1), and vary the Rossby number. We find that rotation gradually suppresses small-scale 3D motions and therefore inhibits vertical transport as Ro decreases towards Fr. The effect is particularly pronounced within the cores of emergent cyclonic vortices. For sufficiently strong rotation, vertical motions are entirely suppressed.

How to cite: Buhl, D., Garaud, P., and Wang, H.: Rotating Stratified Turbulence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7085, https://doi.org/10.5194/egusphere-egu25-7085, 2025.

EGU25-7453 | ECS | Orals | NP6.2

A Lagrangian view of mixing in stratified shear flows 

Xingyu Zhou, John Taylor, and Colm-cille Caulfield

Stratified shear flows are commonplace in the ocean and the atmosphere. Understanding the mechanisms by which such flows become turbulent and lead to irreversible mixing due to the ultimate break down of different types of primary instabilities is vital in understanding diapycnal fluxes of heat and other important scalars such as salt and carbon. We consider numerically the Lagrangian view of turbulent mixing in stably stratified parallel shear flow where both the initial velocity field and initial density departure from the base hydrostatic state have a hyperbolic tangent profile in the vertical coordinate with the same point of inflection. By varying the ratio of velocity interface thickness and density interface thickness, these initial conditions permit two types of instabilities: Kelvin-Helmholtz instability (KHI) and Holmboe wave instability (HWI). These instabilities lead to two distinct types of mixing; overturning motions within the density interface, and scouring by turbulence on the edges of the density interface. Here, we examine mixing from a Lagrangian perspective using direct numerical simulations (DNS) for initial conditions that are unstable to KHI and HWI. Lagrangian particles are tracked in the simulations, and the fluid buoyancy sampled along particle paths provides a Lagrangian measure of mixing. The timing of mixing events experienced by particles inside and outside the interface is different in simulations exhibiting KHI and HWI. The particles exhibit aggregation in buoyancy space when there is sustained overturning motion within the interface. The root mean square (RMS) buoyancy for a set of particles that start with the same buoyancy is larger for HWI than KHI for the same bulk Richardson number, implying heterogeneous mixing along particle paths for HWI. Finally, the number of particles starting close to the mid-plane of the interface which experience a change in sign in the local fluid buoyancy and end on the opposite side of the mid-plane is compared for KHI and HWI for several values of the bulk Richardson number. Surprisingly, for HWI with a large bulk Richardson number, more than half of the particles that start near the mid-plane end on the opposite side of the mid-plane. We explain this result in terms of localisation of mixing.

How to cite: Zhou, X., Taylor, J., and Caulfield, C.: A Lagrangian view of mixing in stratified shear flows, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7453, https://doi.org/10.5194/egusphere-egu25-7453, 2025.

EGU25-11273 | ECS | Posters on site | NP6.2

Understanding Stratified Turbulence and Greenhouse Gas Exchange in the Stable Boundary Layer of the Arctic Atmosphere 

Sanjid Backer Kanakkassery, Mathias Goeckede, and Mark Schlutow

Stratified turbulence is a prominent feature in the Arctic boundary layer, where land surface cooling during the night may induce strong stable stratification. This process significantly alters the transport dynamics of heat, momentum and trace gases, including greenhouse gases , which are critical to understanding Arctic carbon feedback processes. The Arctic is warming at a rate three to four times faster than the global average, threatening to destabilize its permafrost carbon reservoir, which stores about 60% of global soil carbon—an amount three times as large as currently contained in the atmosphere. Accurate estimation of Arctic greenhouse gas fluxes is crucial for understanding the feedback processes between the permafrost carbon cycle and climate, as these processes have the potential to transform the region from a carbon sink into a significant carbon source.

Quantifying greenhouse gas fluxes using the eddy covariance technique, where turbulent vertical fluxes are computed from high-frequency atmospheric data, is particularly challenging under stable stratification, where turbulent mixing is suppressed. This study investigates nighttime greenhouse gas transport dynamics in the Arctic’s stably stratified boundary layer based on Large Eddy Simulation (LES) utilizing the EULAG research model. Site-specific data are incorporated to simulate stable stratification induced by surface cooling.

We employ the "age of air" (AoA) concept, traditionally applied in the stratosphere, to evaluate vertical mixing efficiency in stable conditions. Developing AoA-based methods to interpret the transition from nighttime fluxes to early morning measurements, which are often misinterpreted as outliers, will help to provide new insights into land-atmosphere interactions in the Arctic. These findings contribute to improving Earth System Models (ESMs) and enhance our understanding of Arctic greenhouse gas emissions and their impact on global climate.

How to cite: Kanakkassery, S. B., Goeckede, M., and Schlutow, M.: Understanding Stratified Turbulence and Greenhouse Gas Exchange in the Stable Boundary Layer of the Arctic Atmosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11273, https://doi.org/10.5194/egusphere-egu25-11273, 2025.

EGU25-14086 | Orals | NP6.2

Modelling dispersion in stratified turbulent flows as a resetting process  

Colm-cille Caulfield, Nicoloas Petropoulos, and Stephen de Bruyn Kops

In stably stratified turbulent flows, numerical evidence shows that the horizontal displacement of Lagrangian tracers is diffusive while the vertical displacement converges towards a stationary distribution (Kimura and Herring JFM Vol 328 1996). We develop a stochastic model for the vertical dispersion of Lagrangian tracers in stably stratified turbulent flows that aims to replicate and explain the emergence of such a stationary distribution for vertical displacement. The dynamical evolution of the tracers results from the competing effects of buoyancy forces that tend to bring a vertically perturbed fluid parcel (carrying tracers) to its equilibrium position and turbulent fluctuations that tend to disperse tracers. When the density of a fluid parcel is allowed to change due to molecular diffusion, a third effect needs to be taken into account: irreversible mixing. Indeed, `mixing' dynamically and irreversibly changes the equilibrium position of the parcel and affects the buoyancy force that `stirs' it on larger scales. These intricate couplings are modelled using a stochastic resetting process (Evans and Majumdar, PRL, Vol 106 2011) with memory. We assume that Lagrangian tracers in stratified turbulent flows follow random trajectories that obey a Brownian process. In addition, their stochastic paths can be reset to a given position (corresponding to the dynamically changing equilibrium position of a density structure containing the tracers) at a given rate. The model parameters are constrained by analysing the dynamics of an idealised density structure. Even though highly idealised, the model has the advantage of being analytically solvable. We show the emergence of a stationary distribution for the vertical displacement of Lagrangian tracers, as well as identify some instructive scalings. 

This project received funding from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant Agreement No. 956457 and used resources of the Oak Ridge Leadership Computing Facility at the Oak Ridge National Laboratory, supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC05-00OR22725. S. de B.K. was supported under U.S. ONR Grant number N00014-19-1-2152.

 

How to cite: Caulfield, C., Petropoulos, N., and de Bruyn Kops, S.: Modelling dispersion in stratified turbulent flows as a resetting process , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14086, https://doi.org/10.5194/egusphere-egu25-14086, 2025.

EGU25-15961 | ECS | Posters on site | NP6.2

Energetic consistency and heat transport in rotating Rayleigh Benard convection 

Roland Welter

Parameterization is an essential tool for modeling turbulent convection in general circulation models, yet parameterizations may fail to obey physically consistent principles such as energy conservation.  In this presentation, I will present recent analytical and numerical results regarding the importance of energetic consistency in rotating Rayleigh-Benard convection. Specifically, spectral discretizations of the Boussinesq-Oberbeck equations are considered, and we are able to pinpoint the exact criteria under which a spectral discretization will obey energy balance laws consistent with the PDE.  The energy balance laws are then shown to imply a compact global attractor.  We are also able to show that almost any spectral model which does not satisfy such criteria will exhibit unbounded solutions, which are wildly unphysical.  The dynamics of the energetically consistent models are studied, and particular attention is given to stable values of heat transport, as well as the convergence across models where the models accurately represent the PDE.  Implications for energetically consistent parameterization of convective heat transport will then be discussed. 

How to cite: Welter, R.: Energetic consistency and heat transport in rotating Rayleigh Benard convection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15961, https://doi.org/10.5194/egusphere-egu25-15961, 2025.

EGU25-18183 | ECS | Posters on site | NP6.2

Jet formation in three fluid layers over topography 

Chiara Stanchieri, Joseph Henry Lacasce, Hennes Alexander Hajduk, Michiel L.J. Baatsen, and Henk A. Dijkstra

Zonal (east−west) jets are characteristic of many geophysical and planetary systems. On Jupiter, they manifest as strong zonal flows between its visible bands. In Earth’s atmosphere, similar jets occur near the tropopause. The Antarctic Circumpolar Current (ACC), the only current that travels around the globe, has marked density fronts at the surface, reflecting three distinct zonal jets. These jets are unstable, leading to meandring patterns and generating eddies. As such, the jets play a central role in the dynamics of their respective environments.
This project investigates the formation of jets in the ACC, with a focus on the influence of bottom topography on jet structure.
Two different models are used. Both solve the quasi-geostrophic equations, with three fluid layers. Including a third layer helps isolate the direct effects of the bottom topography and permits instability in the upper two layers.
This research clarifies jet formation and the scales involved, contributing to a better understanding of the dynamics in the ACC. As the ACC connects the three main ocean basins, the work has implications for understanding the ocean’s role in the Earth’s climate system.

How to cite: Stanchieri, C., Lacasce, J. H., Hajduk, H. A., Baatsen, M. L. J., and Dijkstra, H. A.: Jet formation in three fluid layers over topography, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18183, https://doi.org/10.5194/egusphere-egu25-18183, 2025.

EGU25-19040 | ECS | Orals | NP6.2

Wave-wave interactions within a typical internal gravity wave spectrum in the ocean 

Pablo Sebastia Saez, Carsten Eden, Dirk Olbers, and Manita Chouksey

Internal gravity waves (IGWs) shape the ocean through their interactions with e.g. eddies and other waves. These interactions can lead to wave breaking and density mixing, which influence large-scale mean flows. The resulting energy transfers shape the spectral shape of IGWs, which is surprisingly similar throughout the oceans - the universal Garrett-Munk (GM) spectrum. A key mechanism shaping this continuous energy spectrum is nonlinear wave-wave interaction. We study the scattering of IGWs via wave-wave interactions under the weak-interaction assumption, using the kinetic equation derived from a non-hydrostatic Boussinesq system with constant rotation and stratification. The kinetic equation and coupling coefficients derived from Eulerian and Lagrangian equations are identical under the resonance condition. By developing Julia-native numerical codes, we evaluate the energy transfers for resonant and non-resonant interactions, including inertial and buoyancy oscillations. Our findings confirm that resonant triads dominate the energy transfers, while non-resonant interactions are negligible in isotropic spectra but may become relevant in anisotropic conditions. These findings provide convergent results at reduced computational costs, improving the efficiency and reliability of energy transfer evaluations in oceanic IGW spectra.

How to cite: Sebastia Saez, P., Eden, C., Olbers, D., and Chouksey, M.: Wave-wave interactions within a typical internal gravity wave spectrum in the ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19040, https://doi.org/10.5194/egusphere-egu25-19040, 2025.

EGU25-20130 | ECS | Posters on site | NP6.2

The impact of internal wave breaking on benthic-pelagic exchange fluxes in a shallow water configuration  

Manita Chouksey and Soeren Ahmerkamp

Internal wave breaking in shallow water regions is a critical process shaping coastal dynamics, with important implications for benthic exchange fluxes, nutrient cycling, and benthic ecosystems. Despite its potential importance, our understanding of the interactions between internal waves and benthic-exchange processes remains limited, and their quantification continues to be challenging due to the complex, multi-scale, and multi-phase nature of the underlying flow system.

We conceptualize a model to investigate the impact of wave-breaking-induced turbulence on seafloor and associated benthic-pelagic exchange fluxes. Using Large Eddy Simulation in a shallow water configuration, the model captures the interactions between breaking waves, the generated localized pressure gradients and benthic-pelagic exchange with high spatial and temporal resolution. Preliminary results provide valuable insights into the role of internal wave breaking and the resulting small-scale turbulence in driving benthic-pelagic exchange processes. 

How to cite: Chouksey, M. and Ahmerkamp, S.: The impact of internal wave breaking on benthic-pelagic exchange fluxes in a shallow water configuration , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20130, https://doi.org/10.5194/egusphere-egu25-20130, 2025.

EGU25-20207 | Orals | NP6.2

Investigating vertical dependence of turbulence regimes and lateral mixing in the mixed layer from drifter observations in the South Atlantic 

Alexa Griesel, Julia Dräger-Dietel, Anagha Aravind, Emelie Breunig, Ruben Carrasco, Jeff Carpenter, Jochen Horstmann, and Ilmar Leimann

The energy transfers in the meso- to submesoscale regime in the ocean yield both up-scale and down-scale components from a complex pattern of flow structures which impact scale-dependent ocean turbulence and mixing that is not yet correctly parameterised in climate models.
The Walvis Ridge region in the South Atlantic is characterized by strong tidal beams and lies in the path of the Agulhas eddies and hence also features large mesoscale energy with associated submesoscale fronts and filaments.
Here, we quantify lateral mixing in the mixed layer using surface drifter observations from two observational campaigns with a unique deployment of two drifter types at two different depth levels simultaneously, one at the very surface and one at 15m depth. We quantify the contribution of the different motions that show up in the drifter trajectories at various time and space scales ranging from hours to months and 100m to 1000s of km and how they influence the applicability of the eddy-diffusion model.                                    

We find that large scale mean flow removal plays a critical role in achieving convergence in the components of the diffusivity tensor and in the major axis component after diagonalization. Writing the diffusivities as the product of time scales and kinetic energy, the significant anisotropy in the diffusivity tensor is mainly explained by the anisotropy in the Lagrangian integral time scales, while the major axis component of the velocity variance tensor is comparable to the minor axis component. The details of this anisotropy depend on scale. Motions on scales smaller than the Rossby Radius contribute significantly to the diffusivities. We discuss how the results relate to what kind of energy cascade exists at which scale.

How to cite: Griesel, A., Dräger-Dietel, J., Aravind, A., Breunig, E., Carrasco, R., Carpenter, J., Horstmann, J., and Leimann, I.: Investigating vertical dependence of turbulence regimes and lateral mixing in the mixed layer from drifter observations in the South Atlantic, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20207, https://doi.org/10.5194/egusphere-egu25-20207, 2025.

EGU25-21139 | ECS | Posters on site | NP6.2

On the development and stabilisation of symmetrically unstable fronts in the surface mixed layer  

Joshua Pein and Lars Czeschel

Destabilising atmospheric forcing can create regions where potential vorticity (PV) takes the opposite sign of the Coriolis parameter, leading to the onset of symmetric instability (SI)—a hybrid convective-inertial perturbation. SI facilitates energy transfers from geostrophically balanced fronts to turbulent kinetic energy in the oceanic surface mixed layer (SML). Using linear theory and high-resolution Large Eddy Simulations (LES), SI’s role in the PV budget and subsequent restratification of the water column is explored. Spin-down experiments with and without a stratified thermocline below the SML reveal that, in the absence of destabilizing atmospheric forcing, PV fluxes from the ocean interior play a minor role in restratification. Instead, cross-frontal Reynolds stress divergences, driven by SI, generate a secondary circulation that efficiently stratifies the SML through a modified turbulent thermal wind response. SI-induced vertical momentum fluxes also drive frontogenesis, forming sharp non-geostrophic fronts at the SML boundaries. These fronts act as hotspots for vertical PV fluxes, where secondary Kelvin-Helmholtz instabilities (KHI) emerge. The complex interplay between SI and KHI, shaped by turbulent energy dissipation, significantly influences the efficiency of restratification and energy redistribution, with important implications for submesoscale dynamics and parameterisations in climate models.

How to cite: Pein, J. and Czeschel, L.: On the development and stabilisation of symmetrically unstable fronts in the surface mixed layer , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21139, https://doi.org/10.5194/egusphere-egu25-21139, 2025.

EGU25-3059 | Orals | NP6.4 | Highlight

Long-lived Equilibria in Kinetic Astrophysical Plasma Turbulence 

Sergio Servidio

Turbulence in classical fluids is characterized by persistent structures that emerge from the chaotic landscape. We investigate the analogous process in fully kinetic plasma turbulence by using high-resolution, direct numerical simulations in two spatial dimensions. We observe the formation of long-lived vortices with a profile typical of macroscopic, magnetically dominated force-free states. Inspired by the Harris pinch model for inhomogeneous equilibria, we describe these metastable solutions with a self-consistent kinetic model in a cylindrical coordinate system centered on a representative vortex, starting from an explicit form of the particle velocity distribution function. Such new equilibria can be simplified to a Gold–Hoyle solution of the modified force-free state. Turbulence is mediated by the long-lived structures, accompanied by transients in which such vortices merge and form self-similarly new metastable equilibria. This process can be relevant to the comprehension of various astrophysical phenomena, going from the formation of plasmoids in the vicinity of massive compact objects to the emergence of coherent structures in the heliosphere.

M. Imbrogno et al, "Long-lived Equilibria in Kinetic Astrophysical Plasma Turbulence", The Astrophysical Journal Letters 972, L5 (2024)

How to cite: Servidio, S.: Long-lived Equilibria in Kinetic Astrophysical Plasma Turbulence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3059, https://doi.org/10.5194/egusphere-egu25-3059, 2025.

EGU25-3117 | ECS | Orals | NP6.4 | Highlight

Evidence of dual energy transfer driven by magnetic reconnection at sub-ion scales 

Raffaello Foldes, Silvio Sergio Cerri, Raffaele Marino, and Enrico Camporeale

The study of space plasmas at the kinetic scale has seen rapid growth in recent years due to the exponential increase in computational power and more accurate in-situ measurements. Both numerical simulations and observations have revealed a clear transition across ion scales from the magnetohydrodynamic (MHD) to the kinetic regime, characterized by different physical phenomena dominating the turbulent properties and the heating of plasmas. Several studies have associated the so-called ion break with magnetic reconnection, which is considered responsible for injecting energy into this range, thereby driving the sub-ion energy cascade.

In this work, we analyze a 2D3V hybrid-Vlasov simulation of forced plasma turbulence using the space-filtering (or coarse-graining) technique, which allows for a simultaneous investigation of energy transfer properties as a function of scale, space, and time. Using this approach, we quantitatively show, for the first time, that magnetic reconnection in non-collisional plasmas is associated with dual energy transfer across ion scales, bridging the MHD and kinetic regimes. The onset of reconnection events triggers the formation of sub-ion scale turbulent fluctuations and plays a crucial role in the appearance of an inverse energy transfer regime originating at these sub-ion scales.

How to cite: Foldes, R., Cerri, S. S., Marino, R., and Camporeale, E.: Evidence of dual energy transfer driven by magnetic reconnection at sub-ion scales, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3117, https://doi.org/10.5194/egusphere-egu25-3117, 2025.

EGU25-3200 | Orals | NP6.4 | Highlight

Formation of a magnetic coherent structure via the merger of two plasmoids at solar supergranular junctions 

Abraham C.L. Chian, Erico L. Rempel, Luis Bellot Rubio, Milan Gosic, and Yasuhito Narita

Formation of a magnetic coherent structure via the merger of two plasmoids at solar supergranular junctions

 

Abraham C.-L. Chian, Erico L. Rempel, Luis Bellot Rubio, Milan Gosic, and Yasuhito Narita

 

We discuss the formation of a large magnetic coherent structure in a vortex expansion–contraction interval, resulting from the merger of two plasmoids driven by a supergranular vortex observed by Hinode in the quiet-Sun (Chian et al., MNRAS 535, 2436, 2024). Strong vortical flows at the interior of vortex boundary are detected by the localized regions of high values of the instantaneous vorticity deviation, and intense current sheets in the merging plasmoids are detected by the localized regions of high values of the local current deviation. The spatiotemporal evolution of the line-of-sight magnetic field, the horizontal electric current density, and the horizontal electromagnetic energy flux is investigated by elucidating the relation between velocity and magnetic fields in the photospheric plasma turbulence. A local and continuous amplification of magnetic field from 286 G to 591 G is detected at the centre of one merging plasmoid during the vortex expansion–contraction interval of 60 min. During the period of vortex contraction of 22.5 min, the line-of-sight magnetic field at the centre of plasmoid-1 (2) exhibits a steady decrease (increase), respectively, indicating a steady transfer of magnetic flux from plasmoid-1 to plasmoid-2. At the end of the vortex expansion–contraction interval, the two merging plasmoids reach an equipartition of electromagnetic energy flux, leading to the formation of an elongated magnetic coherent structure encircled by a shell of intense current sheets. Evidence of the disruption of a thin current sheet at the turbulent interface boundary layers of two merging plasmoids is presented.

 

How to cite: Chian, A. C. L., Rempel, E. L., Bellot Rubio, L., Gosic, M., and Narita, Y.: Formation of a magnetic coherent structure via the merger of two plasmoids at solar supergranular junctions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3200, https://doi.org/10.5194/egusphere-egu25-3200, 2025.

EGU25-3975 | ECS | Posters on site | NP6.4 | Highlight

A Three - Dimensional Hybrid Simulation Study on the Influence of Magnetosheath Turbulence on Magnetopause Reconnection 

Zemeng Li, Meng Zhou, Yongyuan Yi, and Ye Pang

In this study, the three - dimensional global hybrid simulation method is employed to explore the magnetic reconnection phenomenon at the magnetopause and the influencing mechanism of magnetosheath (MSH) turbulence on it. The characteristics of magnetic reconnection at the magnetopause downstream of quasi - perpendicular shocks and quasi - parallel shocks are emphatically compared, covering aspects such as the occurrence frequency of magnetic reconnection, the distribution pattern of X - lines, and the energy conversion of J·E. Through the operation of the three - dimensional hybrid simulation program and detailed analysis, the differences in magnetic reconnection at the magnetopause under different shock conditions are presented.This research work provides certain insights for accurately defining the complex relationship between MSH turbulence and magnetic reconnection at the magnetopause. It is expected to enhance the understanding of space plasma physical processes to a certain extent. The research results contribute to understanding the mechanism of the effect of turbulence on the magnetic field topology and energy transfer process in the magnetosphere, and provide references for subsequent research in the field of space physics. For the interpretation of satellite observation data and the construction and improvement of relevant theoretical models of magnetospheric dynamics, this study also has certain enlightenment and reference values, hoping to play a role in promoting the coordinated development of theory and practice in this field.

How to cite: Li, Z., Zhou, M., Yi, Y., and Pang, Y.: A Three - Dimensional Hybrid Simulation Study on the Influence of Magnetosheath Turbulence on Magnetopause Reconnection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3975, https://doi.org/10.5194/egusphere-egu25-3975, 2025.

EGU25-4634 | Orals | NP6.4

Electron acceleration in reconnecting and non-reconnecting current sheets in the Earth's quasi-parallel bow shock 

Naoki Bessho, Li-Jen Chen, Michael Hesse, Jonathan Ng, Lynn B. Wilson III, Julia E. Stawarz, and Hadi Madanian

In quasi-parallel shock waves, turbulence occurs in the shock transition region due to instabilities such as the ion-ion beam instability, which eventually bends magnetic field lines and current sheets are produced. There are two types of current sheets in the shock turbulence region: reconnecting current sheets and non-reconnecting current sheets. In the Earth’s bow shock, NASA’s Magnetospheric Multiscale (MMS) has been observing many current sheets, some of which show evidence of magnetic reconnection and energetic accelerated particles. 

 

We study electron acceleration in the Earth’s quasi-parallel bow shock by means of 2D particle-in-cell (PIC) simulation. We discuss differences in properties in reconnecting and non-reconnecting current sheets. Reconnecting current sheets and magnetic islands produced by reconnection show significant heating and energetic particles, and several acceleration mechanisms work in these regions: Fermi acceleration, Hall electric field acceleration, and island betatron acceleration. We also demonstrate that electrons are energized in non-reconnecting current sheets. In some regions in turbulence, an elongated, extending current sheet is formed, and electrons can be accelerated by the perpendicular electric field inside the non-reconnecting current sheet. We compare the efficiency between the acceleration mechanisms in reconnection regions and non-reconnecting current sheets.

How to cite: Bessho, N., Chen, L.-J., Hesse, M., Ng, J., Wilson III, L. B., Stawarz, J. E., and Madanian, H.: Electron acceleration in reconnecting and non-reconnecting current sheets in the Earth's quasi-parallel bow shock, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4634, https://doi.org/10.5194/egusphere-egu25-4634, 2025.

EGU25-6399 | ECS | Posters on site | NP6.4

Quantitative Analysis of Energy Conversion and Anomalous Transport in Kelvin-Helmholtz Instabilities at the Magnetopause 

Zhihong Zhong, Ping Zhong, Meng Zhou, Daniel Graham, Ye Pang, Rongxin Tang, Yuri Khotyaintsev, and Xiaohua Deng

The magnetopause is the boundary where the solar wind interacts with the Earth's magnetosphere, playing a crucial role in the transfer and exchange of mass, momentum, and energy. The Kelvin-Helmholtz instability (KHI) is widely recognized as a key mechanism facilitating plasma transport across the magnetopause. However, direct observational evidence remains lacking. Using high-resolution data from the Magnetospheric Multiscale (MMS) mission, we investigated a KHI event by quantitatively analyzing the energy conversion rate, anomalous flow velocity, and anomalous diffusion coefficient associated with electromagnetic perturbations across various frequency ranges. Our results demonstrate that both the primary KHI and its internal small-scale structures contribute significantly to energy conversion, with the primary KHI producing larger anomalous flows and diffusion coefficients than its internal structures. The peak anomalous diffusion coefficient driven by the KHI (~2 × 10¹⁰ m²/s) is an order of magnitude greater than that induced by lower-hybrid drift waves in the magnetopause reconnection boundary layers. These findings provide quantitative evidence of the critical role played by the KHI and its internal small-scale structures in plasma transport and energy conversion at the flank region of magnetopause.

How to cite: Zhong, Z., Zhong, P., Zhou, M., Graham, D., Pang, Y., Tang, R., Khotyaintsev, Y., and Deng, X.: Quantitative Analysis of Energy Conversion and Anomalous Transport in Kelvin-Helmholtz Instabilities at the Magnetopause, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6399, https://doi.org/10.5194/egusphere-egu25-6399, 2025.

The Kelvin-Helmholtz instability (KHI) at the Earth's magnetospheric flanks plays a critical role in driving plasma dynamics, particularly during northward interplanetary magnetic field periods, in which the KHI is active at the low latitude magnetopause. This instability arises due to the velocity shear between solar wind and magnetospheric plasma, forming vortex structures that drive plasma mixing and magnetic reconnection. These vortices generate turbulence and enable the transfer of energy, momentum, and particles across the magnetopause. As a result, the KHI significantly impacts processes like plasma transport and particle acceleration in planetary magnetospheres. 

To investigate the small-scale physics of these processes, we performed high-resolution two-dimensional (2D) fully kinetic particle-in-cell (PIC) simulations using the ECsim code. ECsim stands out as a PIC code that has the unique property of conserving energy to machine precision, which is essential for accurately modeling physical systems where energy transfer is of prime importance. Our simulations focus on conditions characteristic of the Earth's magnetospheric flanks, where the KHI develops and evolves. By examining different plasma parameters, concentrating on particle velocity distribution functions and temperature anisotropies, we analyze the microphysical processes driving plasma mixing and particle energization, with a particular focus on electron physics, which is captured here in full. 

How to cite: Ferro, S. and Bacchini, F.: Fully Kinetic Simulations of Plasma Transport and Particle Energization Induced by the Kelvin-Helmholtz Instability at the Earth’s Magnetopause, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6474, https://doi.org/10.5194/egusphere-egu25-6474, 2025.

EGU25-6516 | ECS | Posters on site | NP6.4

Evolution of ion distribution functions in ionospheric plasmas perturbed by Alfvén waves 

Dario Recchiuti, Lorenzo Matteini, Luca Franci, Emanuele Papini, Giulia D'Angelo, Piero Diego, Pietro Ubertini, Roberto Battiston, and Mirko Piersanti

It is well known that electromagnetic (EM) processes can affect the trapped population of ionized particles in the Earth’s radiation belts and induce particle precipitations that can be measured by satellites. Moreover, in the last decades, several studies have suggested the concurrent occurrence of energetic particle flux variations (the so-called Particle Bursts, PBs) and ionospheric ELF-VLF electromagnetic activity in correspondence to (or even before) large earthquakes. However, to date, the underlying mechanisms connecting seismic-related electromagnetic processes to satellite-detected particle precipitation events remain elusive. In addition, a comprehensive model capable of explaining observed EM perturbations and PBs is still missing, especially during seismo-related phenomena. The lack of detailed investigation into these processes introduces uncertainties regarding the expected time delay between the two phenomena, which hinders the reproducibility and confirmation of reported findings across different studies, even when employing identical methodologies. Consequently, the temporal distribution of claimed seismo-related phenomena exhibits significant variability.

To address these challenges, we present novel numerical simulations investigating wave-particle interactions within a realistic topside ionospheric plasma environment. A hybrid code was successfully employed to simulate the topside ionosphere, incorporating realistic plasma parameters, including plasma beta and species composition. Simulation results demonstrate some modifications in the ion velocity distribution function, including the emergence of fast ion beams capable of inducing particle precipitation. These simulations provide, for the first time, an estimate of the time delay between the onset of EM waves and the resulting plasma modifications.

How to cite: Recchiuti, D., Matteini, L., Franci, L., Papini, E., D'Angelo, G., Diego, P., Ubertini, P., Battiston, R., and Piersanti, M.: Evolution of ion distribution functions in ionospheric plasmas perturbed by Alfvén waves, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6516, https://doi.org/10.5194/egusphere-egu25-6516, 2025.

EGU25-7607 | Orals | NP6.4 | Highlight

Compression Acceleration of Protons and Heavier Ions at the Heliospheric Current Sheet 

Giulia Murtas, Xiaocan Li, Fan Guo, and Colby Haggerty

Recent observations by Parker Solar Probe (PSP) suggest that protons and heavier ions are accelerated to high energies by magnetic reconnection at the heliospheric current sheet (HCS). In this work I discuss the compression acceleration of protons and heavier ions as a source of energetic particles in the reconnecting HCS, by solving the energetic particle transport equation in large-scale MHD simulations. The multi-ion acceleration results in nonthermal power-law energy distributions, whose spectral index is consistent with PSP observations. Our study shows that the high-energy cutoff of protons can reach Emax ∼ 0.1-1 MeV, depending on the particle diffusion coefficients. The high-energy cutoff of different ion species scales with the charge-to-mass ratio Emax ∝ (Q/M)α, and the particle injection energy can play a role in modifying the scaling factor α, for which we also find a match with the interval α ~ 0.6 - 1.5 observed by PSP.

How to cite: Murtas, G., Li, X., Guo, F., and Haggerty, C.: Compression Acceleration of Protons and Heavier Ions at the Heliospheric Current Sheet, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7607, https://doi.org/10.5194/egusphere-egu25-7607, 2025.

EGU25-8982 | ECS | Orals | NP6.4

Application of the BxC toolkit to the study of cosmic rays transport 

Daniela Maci, Rony Keppens, and Fabio Bacchini

The study of turbulent magnetic fields is crucial in modern astrophysics due to the omnipresence of plasma in a turbulent state. The state-of-the-art approach to the study of turbulence entails the use of numerical simulations, whose high computational cost unfortunately impedes a large variety of studies. To solve this issue, synthetic turbulence models have been developed, in which turbulent fields are generated analytically at a much lower computational cost. 

In the present work we focus on BxC, a Python-based toolkit that generates realistic turbulent magnetic fields through a combination of a geometric and analytical approach. Due to a relatively large set of input parameters, BxC allows for full customization of the statistical properties of the generated fields. Recent developments of the code improve on the possibility to reproduce realistic scenarios, in particular allowing for anisotropic fields and/or ‘structured’ turbulent fields as an alternative to purely turbulent ones.  

In view of practical application of the BxC toolkit, the code has been coupled with the MPI-AMRVAC framework, a parallelized finite-volume solver for partial differential equations. This combined framework has then been applied to the study of cosmic rays transport by means of test particle simulations. The presentation will introduce the audience to the combined approach used, highlighting its advantages and focusing on the results obtained from this study. 

How to cite: Maci, D., Keppens, R., and Bacchini, F.: Application of the BxC toolkit to the study of cosmic rays transport, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8982, https://doi.org/10.5194/egusphere-egu25-8982, 2025.

EGU25-9707 | ECS | Posters on site | NP6.4

Linking Particle Acceleration to Magnetic Reconnection 

Nadja Reisinger and Fabio Bacchini

Magnetic reconnection, a fundamental plasma process, explosively releases energy, generates particles with high energies and plays a crucial role in space weather. This process, which is very common in space plasmas, also occurs in Earth’s magnetotail, driving particle acceleration and affecting the plasma dynamics of the near-Earth space environment. 

To explore the connection between magnetic reconnection and particle acceleration, we present fully kinetic simulations of magnetic reconnection in Earth's magnetotail, including both ions and electrons. For this purpose, we employed the particle in cell (PIC) code ECsim and set up the simulation with parameters from a well-studied magnetic reconnection event observed by the Magnetospheric Multiscale (MMS) mission. This event, usually referred to as a “quiet magnetic reconnection” event, is characterized by less enhanced plasma heating and turbulence.

Our study first compares the particle energization observed in the MMS data with the results from our simulation for this specific reconnection event. By examining the differences and similarities between the two, we aim to evaluate how well the simulation captures the key features of the observed event. Afterward, we vary the initial parameters to investigate how various reconnection scenarios affect particle acceleration. This approach allows us to analyze how different environmental conditions influence the acceleration of particles during magnetic reconnection.

How to cite: Reisinger, N. and Bacchini, F.: Linking Particle Acceleration to Magnetic Reconnection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9707, https://doi.org/10.5194/egusphere-egu25-9707, 2025.

EGU25-12278 | ECS | Posters on site | NP6.4

Fully kinetic and hybrid PIC modelling of magnetosheath turbulence: closure and dissipation 

George Miloshevich, Giuseppe Arrò, Francesco Pucci, Pierre Henri, Giovanni Lapenta, and Stefaan Poedts

Understanding the interactions between the solar wind and the magnetosphere requires multi-scale modelling to resolve magnetohydrodynamic, ion and electron kinetic scales, owing to the collisionless character of plasma turbulence. This leads to computational complexity that reduced models aim to address.

In this study, we investigate decaying turbulence in the magnetosheath by performing comparisons between the ECsim (a fully-kinetic Energy Conserving PIC) model and a computationally lighter model Menura (a hybrid PIC). Menura resolves kinetic ion scales but the influence of massless electrons is provided only via the pressure closure in the generalized Ohm’s law. To ensure meaningful comparisons, we have adjusted the initial conditions using parameters consistent with magnetosheath observations.  

We present a detailed analysis of the pressure-strain interaction terms, electromagnetic work and cross-scales fluxes, demonstrating relatively good agreement between the two models and validating certain turbulent characteristics for Menura. Our findings confirm several established results from fully kinetic Vlasov and PIC simulations, such as connections between coherent structures and energy conversion. Furthermore, we are extending these insights to a novel magnetosheath regime for a hybrid PIC model, which has generally received less attention in such studies. However, discrepancies were also identified, such as Zenitani measure (electromagnetic work done by the non-ideal electric field) and absolute values of energy dissipation which are model-dependent.

In the effort to further improve electron pressure closure, we train a neural network surrogate on ECsim generated data (high fidelity model). We present preliminary results showing consistent scaling for predicted pressure-strain at future simulation time steps as a function of traceless stress, vorticity and the mean square total current density in a lack of data regime.

How to cite: Miloshevich, G., Arrò, G., Pucci, F., Henri, P., Lapenta, G., and Poedts, S.: Fully kinetic and hybrid PIC modelling of magnetosheath turbulence: closure and dissipation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12278, https://doi.org/10.5194/egusphere-egu25-12278, 2025.

EGU25-12337 | ECS | Posters on site | NP6.4

Electron scale magnetic holes generation driven by Whistler-to-Bernstein mode conversion in fully kinetic plasma turbulence 

Joaquín Espinoza Troni, Giuseppe Arrò, Felipe Asenjo, and Pablo Moya

Magnetic holes (MHs) are coherent structures typically observed in turbulent plasmas, characterized by a sharp decrease in the magnetic field magnitude. MHs exist in different sizes, from magnetohydrodynamic to kinetic scales. Magnetospheric Multiscale (MMS) observations have revealed that electron scale MHs are very common in the turbulent Earth’s magnetosheath, potentially playing an important role in the energy cascade and dissipation. Nevertheless, the origin of MHs is still unclear and debated. In this work, we use fully kinetic simulations, initialized with typical Earth's magnetosheath parameters, to investigate the role of plasma turbulence in generating electron scale MHs. We identify a new turbulent-driven mechanism capable of generating MHs at scales of the order of a few electron inertial lengths. This mechanism involves the following steps: first, large-scale turbulent velocity shears produce localized regions with strong perpendicular electron temperature anisotropy; these regions quickly become unstable, producing oblique  whistler waves; then, as whistler fluctuations propagate over the inhomogeneous turbulent background, they develop a quasi-electrostatic component, evolving into Bernstein-like modes; the electric field of Bernstein-like modes produces filamentary electron currents that turn the wave into a train of current vortices; these vortices finally merge into a larger vortex that reduces the local magnetic field magnitude, ultimately evolving into a coherent electron scale MH. This work provides numerical evidence of a turbulence-driven mechanism for the generation of electron-scale MHs. Our results have potential implications for understanding the formation and occurrence of electron scale MHs in the Earth’s magnetosheath and other turbulent environments.

 

How to cite: Espinoza Troni, J., Arrò, G., Asenjo, F., and Moya, P.: Electron scale magnetic holes generation driven by Whistler-to-Bernstein mode conversion in fully kinetic plasma turbulence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12337, https://doi.org/10.5194/egusphere-egu25-12337, 2025.

EGU25-12621 | Posters on site | NP6.4

 Whistler Waves and Electron Deficit in the Solar Wind: Insights from Particle-in-Cell Simulations   

Maria Elena Innocenti, Jesse Coburn, Daniel Verscharen, and Alfredo Micera
In-situ observations of the solar wind reveal that the electron velocity distribution function (VDF) is composed of a quasi-Maxwellian core, which constitutes the majority of the electron population, along with two more sparse components: the halo, consisting of suprathermal and quasi-isotropic electrons, and the strahl, an escaping beam population. Recent measurements by the Parker Solar Probe (PSP) and Solar Orbiter (SO) have identified an additional feature in the non-thermal VDF structure: the deficit—a depletion in the sunward region of the VDF, long predicted by exospheric models but only recently extensively observed.  
Using Particle-in-Cell simulations, we analyze electron VDFs that reproduce those typically observed in the inner heliosphere and explore the potential role of the electron deficit in triggering kinetic instabilities. Prior studies and in-situ data indicate that strahl electrons can drive oblique whistler waves unstable, leading to their scattering. This process enables suprathermal electrons to access phase-space regions that satisfy resonance conditions with parallel-propagating whistler waves.  
The suprathermal electrons lose kinetic energy, resulting in the generation of unstable waves. The sunward side of the VDF, initially depleted of electrons, is gradually filled, as this wave-particle interaction process, triggered by the depletion itself, takes place.
Our results are validated against current PSP and SO observations. Specifically, the study provides insights into the origins of the frequently observed parallel anti-sunward whistler waves in the heliosphere, their correlation with electron-deficit distributions, and a non-collisional process regulating heat flux.  

 

How to cite: Innocenti, M. E., Coburn, J., Verscharen, D., and Micera, A.:  Whistler Waves and Electron Deficit in the Solar Wind: Insights from Particle-in-Cell Simulations  , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12621, https://doi.org/10.5194/egusphere-egu25-12621, 2025.

EGU25-12735 | ECS | Orals | NP6.4

Energy-Conserving Semi-Lagrangian Scheme for Multiscale Plasma Dynamics 

Hongtao Liu and Giovanni Lapenta

Plasma systems exhibit complex multiscale dynamics that require full kinetic models for accurate representation. Explicit kinetic schemes are easy implemented but require time steps finely resolved to the plasma period and suffer from numerical heating, while implicit schemes ensure stability but at the expense of computationally intensive nonlinear solvers. Semi-implicit methods strike a balance between efficiency and stability, but struggle to conserve energy, leading to potential instabilities. While ECSIM introduced a pioneering energy-conserving semi-implicit PIC framework, developing efficient and unconditionally stable grid-based schemes with energy conservation remains a significant challenge.

We propose an inherently noise-free energy-conserving semi-Lagrangian (ECSL) scheme that retains the efficiency of explicit methods and the stability of implicit approaches. Numerical experiments validate its accuracy, efficiency, and energy conservation, demonstrating ECSL as a promising tool for multiscale plasma simulations.

How to cite: Liu, H. and Lapenta, G.: Energy-Conserving Semi-Lagrangian Scheme for Multiscale Plasma Dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12735, https://doi.org/10.5194/egusphere-egu25-12735, 2025.

EGU25-14612 | Orals | NP6.4

In Remembrance of Prof. Giovanni Lapenta 

Jeremiah Brackbill

Italy ended research on Nuclear Energy and in response, nuclear engineering faculty at Politecnico di Torino
placed selected students with established plasma physics groups.  Gianni Lapenta was the first.   He would spend 
half a year with Bruno Coppi at MIT, and half a year with me at Los Alamos.  When I met Gianni,
he said he  liked Boston and Coppi and would prefer to stay there. To my surprise, he arrived in Los Alamos
the following January. 

I suggested a problem to Gianni,   He published his results  in:  G. Lapenta and J U Brackbill, Dynamic and selective control of the number 
of particles in kinetic plasma simulations,  J. Comput. Phys. {\bf{115} }(1994) 213.  In another project with semi-conductor manufacturers, we modeled the deposition of 'dust' on large-scale integrated circuits.   Our results were published in G. Lapenta, F. Iinoya and J. U. Brackbill, "Particle-in-cell simulation of glow discharges in complex geometries," in IEEE Transactions on Plasma Science, vol 23 no. 4, pp. 769-779.  We modeled the interaction of a wafer assembly and the surrounding plasma self-consistently.  Gianni did further work on dust charging in a flowing plasma and published the work in Physical Review Letters.  He modeled  particles that developed dipole moments.  

Gianni became a staff member, a US citizen, and a member of the plasma physics group.  He began to apply the implicit moment plasma simulation code to study magneitic reconnection.  He brought students from Torino, to Los Alamos, among them Paolo Ricci, Stefano Markidis, Jean-Luc Delzanno, and Maria Elena Innocenti., and he published extensively on the lower hybrid instability, colllisionless reconnection, and , later, turbulence.  

In 2008,  he joined the Mathematics Department at KU Leuven  as a professor in Space Weather where he remained until his death in May, 2023.  He continued to  visit the US to work with Maha Abdallah at UCLA and Marty Goldman at the University of  Colorado.  I don't know the full breadth of his work, but I know that he was excited to discover that turbulent flow generated self-sustaining magnetic reconnection.  With Stefano Markidis, he developed a plasma simulation code on  massively parallel computers , and with colleagues at the University of Michigan a method to couple magnetohydrodynamic and kinetic simulation.  My favorite paper appeared in Ap. J. in 2021 on 'Detecting reconnection sites using the Lorentz transformations for electromagnetic fields'.  His method is a simple and reliable way to identify reconnection sites in plasma simulations.

Gianni and I were friends for many years.  We talked when he was diagnosed with cancer.  He was upset by the grim prognosis. So many things he had looked forward to were now out of reach, including a visit with us in Los Alamos.  He died 28 May 2023 at his home in Italy.

How to cite: Brackbill, J.: In Remembrance of Prof. Giovanni Lapenta, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14612, https://doi.org/10.5194/egusphere-egu25-14612, 2025.

EGU25-14631 | ECS | Posters on site | NP6.4

Energy transfer and dissipation of electron current layer during anti-parallel magnetic reconnection 

Dongke Chen, Can Huang, Aimin Du, and Yasong Ge

Magnetic reconnection is often considered to be the most fundamental mechanism for the release of magnetic energy in various plasma systems. Electron current layer (ECL) in the diffusion region plays an important role on energy dispassion during collisionless magnetic reconnection. ECL splits into two sublayers and is maintained at the electron inertial scale, not long after the triggering of anti-parallel magnetic reconnection. By performing 2D particle-in-cell (PIC) simulations with high-resolution grids, we investigate the energy transfer and dissipation of electron current layer during anti-parallel magnetic reconnection. Starting from the energy equation of the two-fluid model, we examine the energy transfer and transports in the vicinity of the ECL through a point-by-point analysis of heating and acceleration, and obtain a new image of the energy conversion in the ECL sublayers. In this work, instead of determining the overall energy budget in a fixed-box, we rather chose to distinguish the diffusion into multiple variational regions to calculate the transfer of energy as the reconnection progressed. By combining calculations based on macroscopic energy equations and analysis of phase space electrodynamics, we find the mechanism of electron thermalization and acceleration in the diffusion region during anti-parallel magnetic reconnection.

How to cite: Chen, D., Huang, C., Du, A., and Ge, Y.: Energy transfer and dissipation of electron current layer during anti-parallel magnetic reconnection, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14631, https://doi.org/10.5194/egusphere-egu25-14631, 2025.

EGU25-17373 | ECS | Posters on site | NP6.4 | Highlight

Reconstructing fluid closures using supervised Machine Learning  

Sophia Köhne, Simon Lautenbach, Emanuel Jeß, Rainer Grauer, and Maria Elena Innocenti

The process of deriving fluid equations from the Vlasov equation for collisionless plasmas involves a fundamental challenge known as the closure problem. This problem consists of the fact that the temporal evolution of any particle moment—such as density, current, pressure, or heat flux—includes terms that depend on the next higher-order moment. Consequently, truncating the description at the nth order necessitates approximating the contributions of the (n+1)th order moment within the evolution equation for the nth moment. The choice of truncation level and the assumptions underlying these approximations play a critical role in determining the accuracy with which the resulting fluid model captures kinetic processes.

The work presented here focuses on reconstructing higher-order moments using only lower-order moments, along with the electric and magnetic fields, as inputs. We apply supervised machine learning to train models that predict higher-order moments, specifically the divergence of the heat flux tensor, in simulations of magnetic reconnection within a Harris current sheet under varying background guide fields. All simulations we use are obtained with the muphy 2 code (Allmann-Rahn et al. 2023). Fully kinetic Vlasov simulations, which provide complete physical information, serve as the ground truth. The reconstructed moments are incorporated into fluid simulations, and their impact on the simulation dynamics is analyzed. We evaluate the models' ability to generalize across different guide field conditions and compare the performance of the machine learning-based closures with commonly used closures in fluid simulations.

How to cite: Köhne, S., Lautenbach, S., Jeß, E., Grauer, R., and Innocenti, M. E.: Reconstructing fluid closures using supervised Machine Learning , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17373, https://doi.org/10.5194/egusphere-egu25-17373, 2025.

EGU25-17592 | Posters on site | NP6.4

Particle-in-cell study of the tearing instability for relativistic pair plasmas 

Kevin Schoeffler, Björn Eichmann, Fulvia Pucci, and Maria Elena Innocenti

Two-dimensional particle-in-cell (PIC) simulations explore the collisionless tearing instability from a Harris equilibrium of a pair (electron-positron) plasma, with no guide field, for a range of parameters from non-relativistic to relativistic temperatures and drift velocities. Growth rates match the predictions of Zelenyi & Krasnosel'skikh (1979) modified for relativistic drifts by Hoshino (2020) as long as the assumption holds that the thickness of the current sheet is larger than the Larmor radius. Aside from confirming these predictions, we explore the transitions from thick to thin current sheets and from classical to relativistic temperatures. We determine a limit for the minimum current thickness to which a current sheet can evolve before the tearing instability sets in. Large-scale astronomical environmental parameters imply significant reconnection of system size current sheets is most likely in regimes with relativistic temperatures, e.g. active galactic nuclei. We also explore the nonlinear evolution of the modes that move to lower wave numbers (especially for thick current sheets with low growth rates) and eventually increase to faster growth rates associated with thinner current sheets before saturating.

How to cite: Schoeffler, K., Eichmann, B., Pucci, F., and Innocenti, M. E.: Particle-in-cell study of the tearing instability for relativistic pair plasmas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17592, https://doi.org/10.5194/egusphere-egu25-17592, 2025.

EGU25-17863 | ECS | Posters on site | NP6.4

Discovering heat flux closures using machine learning methods 

Emanuel Jeß, Simon Lautenbach, Sophia Köhne, and Maria Elena Innocenti

In computational plasma physics kinetic models are used to simulate plasma phenomena where small scale physics is expected to be of importance. These models contain the full information of the particle velocity distribution function but are computationally expensive. Therefore, computationally cheaper models are utilized, which can then be deployed to larger scales e. g. 10-moment fluid models or magnetohydrodynamics (MHD). However, the large scale behavior is critically influenced by small scale behavior. For example, solar wind observations show that ion and electron scale instabilities constrain the solar wind temperature anisotropy over the entire heliosphere (Berčič et al., 2019; Matteini et al., 2013)  and in our group we have recently demonstrated via fully kinetic numerical simulations the non-trivial link between the small and the large scales in heat flux regulation in the solar wind (Micera et al., 2021; Micera et al., 2025). Thus, models are required that can include kinetic processes, in reduced form, into large scale simulations. At the moment, analytical closures are used to close the hierarchy of fluid equations, but these closures are strictly valid only in certain regimes. For example, Landau fluid closures (Hammett & Perkins, 1990; Hunana et al., 2019) assume that the plasma is close to Local Thermodynamic Equilibrium, which is not the case for most space plasmas. Finding suitable closure equations is an ongoing research topic that gets increasingly more difficult in complex systems. In this study, we try to improve fluid models by learning a suitable symbolic closure for the heat flux by applying machine learning methods (Alves & Fiuza, 2022; Long et al., 2019) to data from kinetic simulations.
At first, these methods were tested by learning the lower moment equations using simulation data of the two stream instability.
In the long term, closure equations for more complex systems will be addressed.

How to cite: Jeß, E., Lautenbach, S., Köhne, S., and Innocenti, M. E.: Discovering heat flux closures using machine learning methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17863, https://doi.org/10.5194/egusphere-egu25-17863, 2025.

EGU25-2573 | Orals | NP6.5

On the Spreading of Meltwater Plumes in the Ocean during the Last Deglaciation 

Olivier Marchal and Alan Condron

The dispersal of meltwater discharged from the St. Lawrence Valley is investigated from numerical experiments with a regional configuration of the MIT general circulation model representing the western North Atlantic during the last ice age. These experiments assume a horizontal resolution of 1/20o and a vertical grid with 21 levels in the upper 100 m, so that both the mesoscale eddy field and the vertical structure of the meltwater plume could be simulated in detail. Our goals are to identify possible mechanisms responsible for the offshore spreading of meltwater in the ocean during the deglaciation and to help the interpretation of paleoceanographic observations from the seafloor and sediment cores.

We find that meltwater discharged from the St. Lawrence Valley forms a buoyant plume which turns to the southwest along the continental slope under the action of the Coriolis force. Part of the meltwater is entrained away from the slope by meander crests and warm-core rings of the Gulf Stream (GS) between the St. Lawrence Valley and Cape Hatteras. The other part is diverted offshore by the opposing GS near Cape Hatteras, where the GS leaves the continental margin. In one experiment, meltwater is incorporated into a meander trough that pinches off and produces a cold-core ring, leading to meltwater transport into the subtropical gyre, or it flows southward along the slope inshore of the GS to the South Atlantic Bight. Sensitivity tests show that the buoyant plume spreads at a consistent rate of O(105 m2 s-1). A reduced-gravity two-layer model suggests that the spreading of the plume is governed by (i) the net ageostrophic motion produced by the total acceleration and the upwelling-favorable winds along the front of the plume and (ii) the advection of the front of the plume by the ambient geostrophic flow. In our experiments, meltwater in turn alters the upper part of the GS through meltwater-induced changes in cross-stream density gradients. Our results put constraints on the interpretation of ice-rafted debris found in (de)glacial sediments from the Sargasso Sea and of iceberg scours observed on the slope south of Cape Hatteras.

How to cite: Marchal, O. and Condron, A.: On the Spreading of Meltwater Plumes in the Ocean during the Last Deglaciation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2573, https://doi.org/10.5194/egusphere-egu25-2573, 2025.

EGU25-3131 | Posters on site | NP6.5

Impact of Ice Keel Geometry on Internal Solitary Wave Dynamics 

Kateryna Terletska, Vladimir Maderіch, and Gabin Urbancic

This study explores the transformation processes and energy dissipation of internal solitary waves (ISWs) in the Arctic Ocean under varying ice keel geometries. Using a nonhydrostatic numerical model based on Reynolds-averaged Navier–Stokes equations under the Boussinesq approximation, we simulate the interaction of ISWs with groups of ice keels characterized by different configurations. The computational domain represents a simplified 2D stratified fluid with an idealized vertical density profile mimicking summer conditions on the Yermak Plateau.  The ice keel geometries were parameterized using the Versoria function. The experiments involved ISWs with an amplitude of 20 m interacting with groups of ice keels characterized by varying numbers and lengths.The shapes of the ice keels were designed with common envelopes of differing heights and lengths, incorporating configurations with varying numbers of keels (1, 7, and 13).This approach allows for systematic and consistent comparisons of their effects on wave dynamics, energy dissipation, and the resulting mixing processes within the ocean's stratified layers. These shapes closely approximate the geometry of ice keels studied in the MOSAiC project, which provided valuable observational data and insights into the physical processes governing wave-ice interactions in the polar environment [1].

Key findings indicate significant energy dissipation for ISWs propagating through ice keel fields, with greater losses observed for larger numbers of keels. The highest energy dissipation occurred in cases with 13 keels due to increased reflections and turbulent mixing. Additionally, the interaction of ISWs with multiple keels enhances mixing in the stratified ocean layer beneath the ice. Variations in keel geometry and number intensify turbulence, contributing to a more complex wave field. Furthermore, these interactions generate second-mode internal waves that interact with first-mode waves and other second-mode waves, further intensifying energy dissipation and wave transformation. This mode-mode interaction creates a dynamic wave environment, emphasizing the role of keel morphology in polar ocean mixing.

These findings highlight the importance of ice keel geometry in modulating ISW dynamics and their contribution to upper ocean mixing processes. The study offers valuable insights into wave-ice interactions and their implications for Polar Ocean dynamics, with broader applications for understanding polar mixing processes and their influence on global ocean circulation.

 

[1] Nicolaus, Marcel & Perovich, Donald & Spreen, Gunnar & Granskog, Mats & von Albedyll, Luisa & Angelopoulos, Michael & Anhaus, Philipp & Arndt, Stefanie & Bünger, H. Jakob & Bessonov, Vladimir & Birnbaum, Gerit & Brauchle, Joerg & Calmer, Radiance & Cardellach, Estel & Cheng, Bin & Clemens-Sewall, David & Dadic, R. & Damm, Ellen & Boer, Gijs & Wendisch, Manfred. (2022). Overview of the MOSAiC expedition: Snow and sea ice. Elem Sci Anth. 10. 10.1525/elementa.2021.000046.

 

How to cite: Terletska, K., Maderіch, V., and Urbancic, G.: Impact of Ice Keel Geometry on Internal Solitary Wave Dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3131, https://doi.org/10.5194/egusphere-egu25-3131, 2025.

EGU25-4294 | Posters on site | NP6.5

What controls the structure of turbidity currents? 

Daniela Vendettuoli, Matthieu, J., B. Cartigny, Michael, A. Clare, Esther, J. Sumner, Peter, J. Talling, Koen Blanckaert, Maria Azpiroz–Zabala, Charlie, K. Paull, Roberto Gwiazda, Jinping, P. Xu, Cooper Stacey, Gwyn, D. Lintern, Steve Simmons, Ed, L. Pope, Lewis, P. Bailey, and John Wood

This study analyzes turbidity currents across multiple systems using high-resolution oceanographic datasets and laboratory experiments. By comparing velocity trends throughout the turbidity currents, we identify two end-member types: short surge flows where peak velocity is followed by rapid decay in velocity and sustained flows where peak velocity is followed by a prolonged near constant velocity. Variability is explored across key parameters, including trigger, system type, slope, grain size, and distance offshore. The findings demonstrate that no single parameter explains all observed variations, with only grain size and distance offshore showing some degree of correlation with the type. Improved data quality, particularly on grain size variability within systems and individual flows, will be essential to understand the different types of flows and their relative process.

How to cite: Vendettuoli, D., Cartigny, M. J. B., Clare, M. A., Sumner, E. J., Talling, P. J., Blanckaert, K., Azpiroz–Zabala, M., Paull, C. K., Gwiazda, R., Xu, J. P., Stacey, C., Lintern, G. D., Simmons, S., Pope, E. L., Bailey, L. P., and Wood, J.: What controls the structure of turbidity currents?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4294, https://doi.org/10.5194/egusphere-egu25-4294, 2025.

EGU25-4429 | ECS | Orals | NP6.5

A numerical and experimental investigation of the influence of heat transfer boundary conditions on convective mixing 

Marianne Pons, Gauthier Rousseau, Hessel Adelerhof, Bastien Carde, Mart Giesbergen, Benoit Fond, Sergey Borisov, and Koen Blanckaert

Temperature-induced density variations within fluids drive gravity-driven flows. Such flows occur for example in geophysical processes such as differential cooling or stratification dynamics in lakes. Heat transfer through the boundaries, whether in a lake or in a laboratory flume, can impact flows. The objective of this study is to evaluate numerically and experimentally the effect of these boundary conditions on thermal convective mixing in two different configurations. The first configuration is the thermal convective mixing in a box of water with cooled boundaries. The second configuration is a lock exchange gravity flow.

Numerical simulations were performed using OpenFOAM with a Large Eddy Simulation solver and the Boussinesq approximation for density effects. The sensitivity of the solution to different boundary conditions for heat transfer were analyzed. Experiments rely on an innovative phosphor thermometry technique able to measure spatial patterns of fluid temperature instead of common pointwise measurements. Notably, we introduce a novel approach that combines the use of a laser sheet and high-resolution CMOS sensors operated in a multi gate accumulation mode to extract the temperature pattern.

The choice of appropriate parameters in the boundary condition enabled the accurate representation of the temperature evolution and convective flow patterns observed in the experiments.

How to cite: Pons, M., Rousseau, G., Adelerhof, H., Carde, B., Giesbergen, M., Fond, B., Borisov, S., and Blanckaert, K.: A numerical and experimental investigation of the influence of heat transfer boundary conditions on convective mixing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4429, https://doi.org/10.5194/egusphere-egu25-4429, 2025.

EGU25-4480 | Posters on site | NP6.5

Gravity currents interacting with bottom large-scale roughness 

Claudia Adduce, Maria Rita Maggi, and Giovanni Di Lollo

Gravity currents, driven by density variations caused by gradients in temperature, salinity, or sediment concentration, arise due to hydrostatic imbalances between adjacent fluids. These flows play a pivotal role in a wide range of geophysical and engineering applications, shaping atmospheric, terrestrial, and subaqueous environments. In natural settings, the propagation of gravity currents often encounters uneven topographies, where the dynamics of the dense flow are significantly influenced by topographic features. Recent research has increasingly focused on understanding gravity currents moving through channels obstructed by finite-size patches of obstacles, which adds complexity to their behavior and mixing processes. This experimental study investigates the interaction mechanisms between gravity currents and such obstructions, providing insights into their dynamics and mixing implications through a non-intrusive image analysis technique based on light reflection to evaluate instantaneous density fields.

Laboratory experiments were conducted in a Perspex tank with dimensions of 3 m in length, 0.3 m in height, and 0.2 m in width. An array of rigid plastic cylinders, each with a diameter of 2.5 cm, was placed at a predetermined location spanning the entire width of the channel. The gravity current was reproduced using the lock-release technique with a density difference ∆ρ=6 kg/m³. A total of 12 full-depth lock-exchange experiments were performed to analyze the submergence ratio, i.e. the ratio between the initial current depth and the obstacle height, and the gap-spacing ratio, i.e. the ratio between the spacing of the bottom obstacles and the obstacle height.

The analysis of instantaneous density fields provides valuable insights into the complex dynamics of gravity currents. During the initial slumping phase, the front of the dense current advances at a constant velocity. However, upon reaching the obstacles, the gravity current slows down, leading to the emergence of distinct flow regimes. The evaluation of the density fields enabled a more detailed description of the flow evolution. It was observed that the front of the dense current detaches from the upstream face of each obstacle. In particular, the temporal and spatial evolution of the dimensionless depth-averaged density obtained by integrating the instantaneous density fields below a threshold of 2% excess density revealed significant phenomena near the current front. This region exhibited increased mixing and dilution as the ratio between the initial current depth and the obstacle height increased. Conversely, the influence of the spacing between the bottom obstacles appeared to be less significant.

How to cite: Adduce, C., Maggi, M. R., and Di Lollo, G.: Gravity currents interacting with bottom large-scale roughness, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4480, https://doi.org/10.5194/egusphere-egu25-4480, 2025.

EGU25-8865 | ECS | Posters on site | NP6.5

Hydro-sedimentary processes of a lofting turbidity current revealed by gridded ADCP measurements in the field 

Stan Thorez, Ulrich Lemmin, D. Andrew Barry, and Koen Blanckaert

Hyperpycnal (negatively buoyant) river inflows into lakes or reservoirs plunge upon entry, generating gravity-driven underflows near the bed. When the density excess of these underflows is primarily due to high sediment concentrations, they are referred to as turbidity currents. If these underflows encounter a layer of equal density, they will detach from the bed and intrude into the water column, forming an interflow. In turbidity currents, such underflow-interflow transitions often happen through a process called ‘lofting’, whereby a flow that is initially negatively buoyant undergoes a buoyancy reversal due to sedimentation of particles. Direct observations of lofting are sparse, particularly in the field. As turbidity currents transport various constituents – not only sediment, but also contaminants, nutrients, and oxygen – originating from the river or eroded from the bed, their trajectory and final destination significantly influence the water quality of lakes and reservoirs. The latter highlights the importance of studying flow transitions such as lofting.

Field measurements of the turbidity current fed by the plunging Rhône River in Lake Geneva were conducted using a boat-towed ADCP along a grid of transects. The ADCP backscatter signal was used to achieve a first order estimate for the sediment concentration.

The measured velocity field reveals that in the longitudinal direction the Rhône River turbidity current initially breaks through the Lake Geneva pycnocline, detaches from the bed, rises vertically and intrudes into the pycnocline. Additionally, in the transverse direction the outermost parts of the current peel off and similarly rise and intrude into the pycnocline. This infers the presence of lofting in both longitudinal and transverse direction. In man-made dammed-river reservoirs, river valley walls provide a high degree of transverse confinement for turbidity currents, which might suppress the development of flow processes in transverse direction, such as transverse lofting. In most natural lakes, such confinement is not present. This infers a potentially significantly different underflow-interflow transition mechanism and resulting morphological impact between reservoir and lake settings.

The estimated sediment concentrations uncover a capacity of the lofting current to transport sediment-rich water away from the turbidity current centerline in transverse direction. This might influence the local bathymetry and support levee-building.

How to cite: Thorez, S., Lemmin, U., Barry, D. A., and Blanckaert, K.: Hydro-sedimentary processes of a lofting turbidity current revealed by gridded ADCP measurements in the field, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8865, https://doi.org/10.5194/egusphere-egu25-8865, 2025.

EGU25-9181 | ECS | Posters on site | NP6.5

Characteristics of turbidity current events in Lake Geneva, Switzerland 

Xiguo Zhang, Stan Thorez, D. Andrew Barry, Ulrich Lemmin, and Koen Blanckaert

Turbidity currents represent a distinctive type of subaqueous density currents, characterized by a density excess that is due to the sediment load. Turbidity currents are important in lakes, reservoirs and oceans and have implications on hazard management, reservoir sedimentation and water quality. The existence of turbidity currents has been inferred in the 19th century from the existence of canyons on lake bottoms and in the 20th century from successive cable breaks of telecommunication cables on the ocean floor. From the 1990s on, Acoustic Doppler Current Profiler’s (ADCP) have allowed measuring vertical profiles of the velocity in turbidity currents. Most measurements were made in oceanic environments, however, and detailed measurements in lakes remain very scarce.

This study reports field measurements of turbidity currents in Lake Geneva, Switzerland, performed in 2016, 2017, 2018 and 2022. The measurements cover a broad range of control parameters and include an entire hydrological year. Additional data were obtained from simultaneous measurements with high-resolution thermistors in vertical profiles or along the lake bottom.

A total of twenty one turbidity current events were identified over the measurement period. For each event, characteristics such as the average and maximum flow velocity, the height, the duration and the dispatched volume of water were extracted from the ADCP velocity record. In addition, the suspended sediment concentration was estimated from the ADCP backscatter record and yielded estimations of the dispatched sediment volume.

The twenty one turbidity currents can essentially be separated in three classes: strong short-term events with velocities above 1 m s-1 that last up to approximately 24 hours, weak long-term events with velocities below 0.3 m s-1 that last several days, and weak short-term events with velocities below 1 m s-1 that last less than 12 hours.

How to cite: Zhang, X., Thorez, S., Barry, D. A., Lemmin, U., and Blanckaert, K.: Characteristics of turbidity current events in Lake Geneva, Switzerland, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9181, https://doi.org/10.5194/egusphere-egu25-9181, 2025.

EGU25-9640 | ECS | Orals | NP6.5

Effect of inflow channel aspect ratio on the plunging dynamics of an unconfined hyperpycnal plume over a sloping bed 

Kingsley Obinna Eze, Antonio Ammendola, George Giamagas, Stan Thorez, Eletta Negretti, Julien Chauchat, and Koen Blanckaert

Hyperpycnal (denser) river inflows into lakes bring sediments, nutrients, oxygen and contaminants, which are crucial for the water quality. Due to the higher densities of hyperpycnal inflows, they abruptly descend toward the lake bottom upon entering the lake, a process called plunging, and subsequently continue flowing along the lake bottom as a gravity-driven underflow. This plunging is accompanied by mixing and entrainment of ambient lake waters, which causes dilution of the initial density excess of the river inflow. The mixing is parameterized by the plunging mixing coefficient Ep  and is of critical importance as it conditions the fate and final destination of the contaminants carried by the river inflows. A recently proposed conceptual model (Thorez et al. 2024) for the plunging into an unconfined lake configuration highlights the importance of the lateral slumping motion of the river plume and secondary flow cells on each side of the plume with respect to the plunging mixing.

This study builds on previous research that suggests that Ep  is affected by the geometry of the river mouth. We investigate with Particle Image Velocimetry (PIV) in laboratory experiments how the width-to-depth ratio at the river mouth (W0H1) influences the plume hydrodynamics and Ep. Four different ratios, W0H1 = 5.4, 9, 13.5 and 27, were investigated in a configuration that mimics the Rhône inflow into Lake Geneva. The laboratory experiments were performed in the Coriolis platform at LEGI (Laboratoire des Ecoulements Géophysiques et Industriels) at a scale of 1:60 that allows minimal scaling effect.

The distance of the plunge location from the river mouth, xp, and the corresponding depth, hp, were found to decrease with the aspect ratio. In addition, the size of the secondary flow cells on each side of the slumping river plume decreased with aspect ratio which tentatively explains the observed variations in Ep.

How to cite: Eze, K. O., Ammendola, A., Giamagas, G., Thorez, S., Negretti, E., Chauchat, J., and Blanckaert, K.: Effect of inflow channel aspect ratio on the plunging dynamics of an unconfined hyperpycnal plume over a sloping bed, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9640, https://doi.org/10.5194/egusphere-egu25-9640, 2025.

EGU25-9685 | ECS | Posters on site | NP6.5

Seafloor dynamics: sediment-ocean interactions in the Diamantina Fracture Zone (SE Indian Ocean) 

Xun Yang, Xiaoxia Huang, Hanyu Zhang, and Xiaotong Peng

Diamantina Fracture Zone in the SE Indian Ocean is one of the less unexplored hadal zones (>6000 m) of our planet without human visits until recently. This study incorporates shallow sediments, submarine videos, and multibeam bathymetry data at a wide range of water depth and geomorphology to fully assess the sediment dynamics of the Diamantina Fracture Zone and their major causative factors. Grain size and organic geochemical analyses confirmed a primary marine source. Australian terrigenous input was indicated by an increasing silty contribution to the eastern hadal section of the fracture zone. Importantly, in the western to middle section, angular volcanic-rich sediments with a peak at 200-300 μm covered the underlying fine pelagic sediments and calcareous oozes, which were likely initiated during the Last Glacial Maximum. Susceptibility to slope failure was high due to localized topographical constraints, rather than earthquakes. The occurrence of sediment ripples at the west and densely-covered manganese nodules at the east implied the ocean bottom circulation with increasing current intensity, which also enhanced the possibility of the gravity-driven slope deposition. This research provides the first knowledge of the highly spatial heterogeneity of sediment dynamics in the remote deep Indian Ocean where continuous but fluctuating downslope and alongslope processes were developed.

How to cite: Yang, X., Huang, X., Zhang, H., and Peng, X.: Seafloor dynamics: sediment-ocean interactions in the Diamantina Fracture Zone (SE Indian Ocean), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9685, https://doi.org/10.5194/egusphere-egu25-9685, 2025.

The South China Sea (SCS) is one of the largest marginal seas on Earth, located at the convergence of the Eurasian, Pacific, and Indo-Australian plates. The basin formed through seafloor spreading during the Oligocene to Middle Miocene and has since been undergoing eastward subduction beneath the Philippine Sea Plate. This process has led to the gradual enclosure of the SCS since the Late Miocene. The region's dynamic tectonic setting, coupled with a tropical typhoon-prone climate, has contributed to the formation of numerous supercritical turbidity current (TC) bedforms within the SCS.

Supercritical bedforms have been documented at more than 20 sites in the SCS, including bedform trains found along canyon/channel thalwegs, as well as bedform fields in unconfined environments like levees, overbank or interfluvial areas, and fans at canyon mouths. The bedform trains along thalwegs typically consist of 5-19 bedforms and vary in length from a few kilometers to ~100 km. The unconfined bedform fields may contain several to over 30 rows of bedforms, covering areas ranging from 176 to 20,000 km². Both the confined and unconfined bedforms are considered supercritical based on their diagnostic morpho-depositional characteristics, including upslope migration, and backset dominant bedding, and erosional truncations on the lee side. The turbidite-dominated sediment components, crest orientation parallel to local isobaths, and their occurrence in canyons/channels and related environments, all suggest formation by TC rather than contour or other bottom currents.

Individual supercritical bedforms in the SCS can be identified as one of the two end members: cyclic steps and antidunes. Cyclic steps show upslope or downslope asymmetry, step-like morphology, and typical downstream-thinning backsets. Antidunes have symmetrical cross-sections, convex-upward structures, downstream-thickening backsets, and, when occurring with cyclic steps, smaller dimensions and aspect ratios. Occasionally, antidunes are superimposed on the stoss side of cyclic steps, identified as chutes-and-pools, representing a transitional type between antidunes and cyclic steps. Both confined and unconfined bedforms exhibit a wide range of wavelengths and wave heights, varying from smaller bedforms with wavelengths of 200-300 m and wave heights of several meters, to larger bedforms with wavelengths typically in the range of kilometers and wave heights reaching tens of meters or more. Confined bedforms are dominated by erosional to partially depositional cyclic steps, or by partially depositional antidunes. Unconfined bedforms are predominantly composed of fully to partially depositional cyclic steps and antidunes, with erosional cyclic steps and chutes-and-pools forming locally. In both cases, depositional bedforms are the most prevalent, likely due to high sedimentation rates resulting from the combined effects of rapid post-rift subsidence and ample sediment supply in the SCS. The widespread presence of supercritical bedforms highlights the important role that supercritical TCs play in SCS’s deep-water sedimentation.

This work was supported by the National Key Research and Development Program of China (2022YFF0800503) and the National Natural Science Foundation of China (91028003, 41676029, and 41876049). 

How to cite: Zhong, G.: Supercritical turbidity-current bedforms in the South China Sea: An overview, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10010, https://doi.org/10.5194/egusphere-egu25-10010, 2025.

EGU25-17431 | ECS | Posters on site | NP6.5

Mixing of tracers in stratified sheared flows      

Marie Andrieux, Yves Morel, Francis Auclair, Yvan Dossmann, Jared Penney, and Peter Haynes

Understanding small-scale turbulent mixing in the ocean is fundamental for accurately modeling oceanic processes, predicting currents, and managing marine ecosystems. Global and regional ocean models rely on parameterizing turbulent mixing, yet this remains a significant source of uncertainty due to technical constraints and model-specific empirical assumptions. Furthermore, when coupled with biogeochemical models, a uniform mixing parameterization is typically applied to all tracers, overlooking the distinct properties of each. This study investigates the influence of turbulent mixing on macroscopic scales and examines the role of molecular diffusion coefficients, which are intrinsically the only irreversible processes affecting passive tracers. Using the CROCO model in a non-hydrostatic, compressible configuration, we conduct direct 3D numerical simulations of turbulence and mixing driven by Kelvin-Helmholtz instabilities. The analysis is based on tracking the properties of fluid particles in a tracer-density space and calculating an effective diffusion coefficient to quantify how fine-scale mixing impacts larger scales redistribution of tracer. The macroscopic scale is associated with the adiabatic rearrangement of the 3D density field into a stable 1D profile, following Lorenz rearrangement. The evolution of these 1D profiles, which only occurs during irreversible mixing, forms the basis for calculating the effective diffusion coefficient. Both theoretical considerations and numerical results in simplified configurations demonstrate that when the molecular diffusion coefficients for tracers and density are equal, the macroscopic effective diffusivity deduced from the density field can be applied to the passive tracer. To evaluate this principle of equality of macroscopic diffusivity, we conduct an experimental study of a gravity current in a large tank (3x0.15x0.2 meters) using a dual light attenuation technique to simultaneously observe the density and passive tracer fields. The same domain is simulated in the numerical model, enabling direct comparisons of mixing dynamics between experimental and numerical gravity currents. Results highlight the critical role of transverse instabilities in driving irreversible mixing. The latter locally modify mixing at macroscopic scale and possibly alter the equality principle. 

How to cite: Andrieux, M., Morel, Y., Auclair, F., Dossmann, Y., Penney, J., and Haynes, P.: Mixing of tracers in stratified sheared flows     , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17431, https://doi.org/10.5194/egusphere-egu25-17431, 2025.

EGU25-17770 | ECS | Orals | NP6.5

Near-field plunging dynamics of laterally unconfined hyperpycnal plumes over inclined beds 

Georgios Giamagas, Cyrille Bonamy, Koen Blanckaert, and Julien Chauchat

The flow of a hyperpycnal river plume into a lake with an inclined bed and without any lateral confinement is a common occurrence in nature.  A characteristic example of such geophysical fluid flow system is the one of  sediment-laden dense river inflows in freshwater lakes (e.g. river Rhone - lake Geneva). In this case, the plunging process close to the river mouth, as well as its dependence on the properties of the inflow, affect critically the subsequent hydrodynamics in the lake. A better understanding of these flow processes is therefore significant for the effective management of the lake water quality and overall ecology. In this talk, we focus on the complex near-field plume dynamics and establish novel criteria for plunging, based on Large Eddy Simulations (LES) of an unconfined hyperpycnal saline plume over an idealized bed. More specifically, we focus on the effect of the variation of the inflow densimetric Froude number, Frd, which is the non-dimensional parameter describing the ratio between inertial and buoyancy forces acting on the plume. In particular, three simulations were performed at different values of Frd, within the range of values encountered in the plunging of river Rhone in lake Geneva. It is found that the near-field dynamics of the hyperpycnal plume is different in the unconfined plunging scenario compared to the case where the flow is confined by lateral walls and that it critically depends on Frd. Indeed, it is a well-established result that in the confined case the plunging of the hyperpycnal plume occurs at the location downstream where a balance between dynamic pressure forces (inertia) and the resisting hydrostatic pressure forces (gravity) is obtained. However, in absence of any lateral confinement the plunging begins immediately upon the entrance of the dense river water in the lake, due to lateral slumping. The slumping takes place at both lateral sides of the plume in the form of a collapse of the dense water column followed by a spread across the lake bottom that is very similar to a lock-release flow configuration. This results in an earlier departure of the plume from the lake surface in the unconfined case compared to the confined case under similar inflow conditions. We are able to determine the effect of Frd on the plunge curve, as well as the extend of the plunging zone on the lake bed, before the plume turns into a gravity current and continues its propagation down the slope. In addition, an explanation is provided for the field observations of surface leakage, where sediment-rich water is detected at the lake surface even downstream of the plunge curve. This explanation focuses on the effect of Frd on the dynamics of the turbulent mixing layers that develop at the interface between the incoming river water and the surrounding lake water. These mixing layers facilitate a substantial transfer of mass and momentum from the inflowing river water to the ambient lake water.

How to cite: Giamagas, G., Bonamy, C., Blanckaert, K., and Chauchat, J.: Near-field plunging dynamics of laterally unconfined hyperpycnal plumes over inclined beds, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17770, https://doi.org/10.5194/egusphere-egu25-17770, 2025.

EGU25-18513 | ECS | Orals | NP6.5

New insights into experimental stratified flows obtained through a physics-informed neural network 

Adrien Lefauve, Lu Zhu, Xianyang Jiang, Rich Kerswell, and Paul Linden

We develop a physics-informed neural network (PINN) to significantly augment state-of-the-art experimental data of stratified flows. A fully connected deep neural network is trained using experimental data in a salt-stratified inclined duct (SID) experiment. SID sustains a buoyancy-driven exchange flow for long time periods, much like an infinite gravity current. The data consist of time-resolved, three-component velocity fields and density fields measured simultaneously in three dimensions at Reynolds number= O(10^3) and at Prandtl or Schmidt number = 700 [1]. The PINN enforces incompressibility, the governing equations for momentum and buoyancy, and the boundary conditions at the duct walls. These physics-constrained, augmented data are output at an increased spatio-temporal resolution and demonstrate five key results: (i) the elimination of measurement noise; (ii) the correction of distortion caused by the scanning measurement technique; (iii) the identification of weak but dynamically important three-dimensional vortices of Holmboe waves; (iv) the revision of turbulent energy budgets and mixing efficiency; and (v) the prediction of the latent pressure field and its role in the observed asymmetric Holmboe wave dynamics. These results mark a significant step forward in furthering the reach of fluid mechanics experiments, especially in the context of stratified turbulence, where accurately computing three-dimensional gradients and resolving small scales remain enduring challenges.

References
[1] L. Zhu, X. Jiang, A. Lefauve, R. R. Kerswell, and P. F. Linden. New insights into experimental
stratified flows obtained through physics-informed neural networks. J. Fluid Mech., 981:R1, 2024.

How to cite: Lefauve, A., Zhu, L., Jiang, X., Kerswell, R., and Linden, P.: New insights into experimental stratified flows obtained through a physics-informed neural network, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18513, https://doi.org/10.5194/egusphere-egu25-18513, 2025.

EGU25-18582 * | ECS | Orals | NP6.5 | Highlight

Towards a numerical configuration of the Strait of Gibraltar at the laboratory scale: The HERCULES project 

Bastien Gouhier, Lucie Bordois, Francis Auclair, Cyril Nguyen, Axel Tassigny, Stef Bardoel, Louis Gostiaux, and Maria Eletta Negretti

The Strait of Gibraltar is the site of a rich and complex physics where flows of different densities interact with a strongly rugged topography. These interactions produce many small-scale processes such as the development of hydraulic jumps, shear instabilities, internal solitary waves, which induce strong mixing and impact the Mediterranean outflow water masses. The dynamics of this gravity current emerging from the Strait and flowing along the canyons of the Gulf of Cadiz is conditioned by its prior evolution inside the Strait. In turn, this dense gravity current plays a crucial role on the large-scale oceanic circulation as it mixes with overlying North Atlantic waters thus modifying the properties of the deep-water masses and therefore, likely the regional and basin-scale circulations. Better understanding and describing these small-scale processes is essential to improve operational oceanic models and climate models since they occur below the grid scale of these models and therefore require parameterizations. Recently, the LEGI team has implemented a realistic setup of the Strait of Gibraltar with the adjacent Gulf of Cadiz and Alboran Sea on the Coriolis Platform at Grenoble, including the barotropic forcing (tide), the baroclinic one (lock-exchange), the Earth’s rotation and a realistic topography. The aim is to bring a better understanding of the small-scale physics which take place in this area. In addition to this experimental approach, centimetric resolution of hydrostatic and non-hydrostatic numerical simulations at the laboratory scale were carried out using the numerical code CROCO (Coastal and Regional Ocean COmmunity model – https://www.croco-ocean.org). A specificity of this code is to be able to efficiently resolve sub-mesoscale processes and to relax both the hydrostaticity and Boussinesq assumptions using a non-hydrostatic and compressible Navier-Stokes solver. The purpose of this numerical approach is manifold: explore ranges of parameters that could not be studied experimentally, develop diagnostic tools, investigate the impact of non-hydrostatic effects, evaluate numerical schemes and parameterizations, investigate more specifically each physical process. However, setting up such a realistic numerical configuration is challenging. For example, if we are interested in the purely barotropic forcing, it is essential to represent the tidal forcing identically as in the experiment. Likewise, when we focus on the purely baroclinic forcing, the inherent steep slopes related to the experimental setup put strong constraints on the numerical code. From these numerical simulations, non-hydrostatic effects on the gravity current dynamics are estimated and analyzed at the laboratory scale. They significantly modify hydraulic jumps formation, overflow transport and deep waters circulation in the Gulf of Cadiz. Boundary conditions, vertical resolution, explicit and implicit vertical mixing or viscous effects are all numerical factors that influence gravity current dynamics. All these features must be carefully studied since they impact both the fate of the Mediterranean waters when they flow into the Atlantic Ocean and the fate of the Atlantic waters flowing into de Mediterranean basin. The aim of this presentation is to present the work carried out up to date in the development of these numerical configurations and to present the associated preliminary results.

How to cite: Gouhier, B., Bordois, L., Auclair, F., Nguyen, C., Tassigny, A., Bardoel, S., Gostiaux, L., and Negretti, M. E.: Towards a numerical configuration of the Strait of Gibraltar at the laboratory scale: The HERCULES project, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18582, https://doi.org/10.5194/egusphere-egu25-18582, 2025.

EGU25-19603 | Orals | NP6.5

Tracking the Mediterranean Outflow from the Bosphorus to the Continental Shelf Edge 

Tulay Cokacar, Hüsne Altıok, Mustafa Yücel, and Hasan Örek

The Mediterranean outflow from the Bosphorus advances through channels and delta features, reaching the shelf edge, spreading across the mid-shelf slope, and cascading down the steep continental slope. During the July 2024 cruise, intensive sampling along transects using CTD and Scanfish provided high-resolution data to better understand the pathways of the Mediterranean plume along the continental slope. This study explores the steering of Mediterranean streams through a complex channel network on the shelf, the evolution of distinct water properties—including dissolved oxygen content—and the eventual transition of the Mediterranean flow into neutrally buoyant layers.

To complement the observational data, the dynamics of the gravity current along the shelf-slope region of the Black Sea, characterized by anomalous temperature and oxygen levels were modeled. Model parameters were optimized and validated against the collected cruise data. These new hydrographic observations and modeling efforts shed light on the Mediterranean gradient flow's penetration into the Black Sea interior, advancing our understanding of its pathways and influence on regional water properties.

How to cite: Cokacar, T., Altıok, H., Yücel, M., and Örek, H.: Tracking the Mediterranean Outflow from the Bosphorus to the Continental Shelf Edge, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19603, https://doi.org/10.5194/egusphere-egu25-19603, 2025.

EGU25-20195 | Orals | NP6.5

3D two-phase flow simulations of lock-release turbidity currents 

julien chauchat, Manohar sharma, Marie Rastello, Cyrille Bonamy, Cyril Gadal, Yvan Dossmann, Matthieu Mercier, and Laurent Lacaze

In this contribution, we present 3D two-phase flow simulations of lock-release turbidity currents using sedFOAM. The Large Eddy Simulation is used for the turbulence modeling while the granular stresses are modeled using a frictional-collisional kinetic theory including interparticle friction (Chassagne et al., 2023). Simulations are performed for different bed slopes, initial volume fractions and particle diameter and density. The numerical results are compared with experiments in terms of front propagation and current shape (Gadal et al., 2023). The simulation results are further used to infer the mechanisms controlling the current attenuation, i.e. the current propagation speed reduction with time. We further use the model to analyse the influence of the flume geometry, free surface versus rigid roof.

How to cite: chauchat, J., sharma, M., Rastello, M., Bonamy, C., Gadal, C., Dossmann, Y., Mercier, M., and Lacaze, L.: 3D two-phase flow simulations of lock-release turbidity currents, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20195, https://doi.org/10.5194/egusphere-egu25-20195, 2025.

EGU25-20409 | ECS | Orals | NP6.5

Buoyancy-driven Flows in Cryospheric Aquatic Systems 

Hugo N. Ulloa, Gustavo Estay, Zhukun Wang, and Daisuke Noto

Buoyancy-driven flows play a fundamental role in shaping the dynamics of cryospheric aquatic systems, including ice-covered and proglacial lakes. These flows, driven by density contrasts resulting from variations in temperature, salinity, or meltwater input, regulate critical processes such as heat transport, nutrient distribution, and ice-ocean interactions. This study investigates the mechanisms underlying buoyancy-driven flows, their variability across diverse cryospheric settings, and their implications for heat and mass redistribution in aquatic systems. By integrating field observations, laboratory experiments, and numerical modeling, we explore the patterns of buoyancy-driven flows and their sensitivity to changing environmental conditions. Our findings emphasize the importance of convective dynamics and the nonlinear equation of state of water in governing heat exchange at solid-liquid interfaces, water column stratification, and localized mixing layers. This research enhances our understanding of fragile aquatic systems and provides new insights into the physics of the cryosphere.

How to cite: Ulloa, H. N., Estay, G., Wang, Z., and Noto, D.: Buoyancy-driven Flows in Cryospheric Aquatic Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20409, https://doi.org/10.5194/egusphere-egu25-20409, 2025.

EGU25-21856 | ECS | Posters on site | NP6.5

Temperature imaging of buoyancy-driven flows using lifetime-based laser-induced phosphorescence of particles 

Gauthier Rousseau, Marianne Pons, Hessel Adelerhof, Mart Giesbergen, Bastien Carde, Benoit Fond, Sergey Borisov, and Koen Blanckaert
Recent advancements in fluid experimentation have made it possible to visualize local temperature in flows by observing the response of photoluminescent dye or particles to light excitation. This has sparked increased interest in exploring laboratory-scale density currents induced by temperature differences. However, unlike the commonly investigated saltwater-freshwater or turbidity currents, heat transfer through boundaries can occur, potentially influencing the dynamics of the buoyancy-driven current.
In this study, we utilize the luminescence lifetime dependence on ambient fluid temperature of phosphor micrometric particles (YAG:Cr) and dye (Zr(PDP)2), to spatially and temporally resolve gravity currents such as lock-exchange flows. Notably, we introduce a novel approach by demonstrating the use of CMOS sensors coupled with an accumulation technique to extract temperature information from high resolution images. This method holds promise as it significantly enhances the accessibility of temperature imaging techniques for experimenters. This innovative approach is adaptable to various experimental setups studying thermal convection in fluid bodies.

How to cite: Rousseau, G., Pons, M., Adelerhof, H., Giesbergen, M., Carde, B., Fond, B., Borisov, S., and Blanckaert, K.: Temperature imaging of buoyancy-driven flows using lifetime-based laser-induced phosphorescence of particles, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21856, https://doi.org/10.5194/egusphere-egu25-21856, 2025.

EGU25-3330 | Posters on site | ST1.11

The Thermodynamic Impact of Compressive Fluctuations on the Solar Wind in the Inner Heliosphere 

Jesse Coburn, Daniel Verscharen, Anna Tenerani, and Christopher Owen

The solar wind plasma is observed to fluctuate over a broad range of space and time scales, extending from scales above the magnetic field correlation scale to below those associated with the particle gyration. At scales larger than the gyroscale, the fluctuations are typically categorised as 1) non-compressive fluctuations that have Alfvénic correlation, 2) compressive fluctuations that perturb the plasma density and pressure. While the amplitude of the compressive fluctuations are subdominant to the Alfvénic component, they have unique dynamics that drastically alter the plasma. For example, compressive fluctuations perturb the pressure anisotropy and beam drift speeds. This may drive the perturbed plasma unstable, generating microscale waves that scatter particles and alter the effective mean free path. In addition, compressive fluctuations perturb the magnetic field strength, leading to stochastic heating and transit time damping. Therefore, an understanding of compressive fluctuations is vital to a complete picture of the plasma thermodynamics. To build on our understanding of the solar wind in the inner heliosphere, we combine observations from Solar Orbiter, Parker Solar Probe, and the Wind spacecraft to study compressive fluctuations. We compare amplitude ratios and polarisations to numerical models to understand the efficiency of various generation mechanisms of compressive fluctuations and how they heat and modify the thermodynamics of the solar wind plasma.

How to cite: Coburn, J., Verscharen, D., Tenerani, A., and Owen, C.: The Thermodynamic Impact of Compressive Fluctuations on the Solar Wind in the Inner Heliosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3330, https://doi.org/10.5194/egusphere-egu25-3330, 2025.

Solar Orbiter observations provide an unprecedented opportunity to study plasma turbulence in the solar wind. On magnetohydrodynamic scales intermittent structures mediate the cascade, due to non-linear wave-wave interactions and coherent structures. Those coherent structures are often quantified and identified by the Partial Variance Increment (PVI).

We obtain magnetic field fluctuations from observations of homogeneous turbulence by wavelet decompositions which preferentially resolve either signatures of coherent structures or wave-packets. Comparing the PVI obtained from both wavelet decompositions, this provides a new, physics based method to determine the PVI threshold above which fluctuations may be coherent structures.

We find a single PVI threshold in each of the kinetic and inertial ranges above which coherent structures typically dominate. This threshold is insensitive to the plasma conditions or heliocentric distance. Therefore, it suggests a ubiquitous constraint on the turbulent phenomenology. This can inform estimates of the heating rates of the solar wind due to the turbulence.

How to cite: Bendt, A. and Chapman, S.: Ubiquitous threshold for coherent structures in the kinetic and inertial ranges of solar wind turbulence from Solar Orbiter observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3592, https://doi.org/10.5194/egusphere-egu25-3592, 2025.

EGU25-3759 | Orals | ST1.11 | Highlight

Turbulent small-scale kinematic dynamo in the terrestrial magnetosheath 

Zoltán Vörös, Owen Wyn Roberts, Yasuhito Narita, Yordanova Emiliya, Rumi Nakamura, Daniel Schmid, Adriana Settino, Martin Wolwerk, Cyril Simon Wedlund, Ali Varsani, Luca Sorriso-Valvo, Philippe André Bourdin, and Árpád Kis

Space plasma turbulence incorporates multi-scale coexisting occurrences of many physical phenomena such as waves, large amplitude field and plasma fluctuations, formation of coherent structures and the large variety of associated energy transfer, transport and conversion processes. For example, magnetic reconnection converts magnetic energy to kinetic and thermal energies and accelerates particles. Contrarily, dynamo action refers to energy conversion processes through which magnetic fields are generated or/and amplified at the expense of kinetic energy. Magnetic reconnection has been extensively studied on the basis of in-situ measurements at large-scale magnetospheric boundaries, in the turbulent magnetosheath and in the solar wind. Dynamo processes have been investigated mainly through numerical studies and in laboratory liquid metal and laser experiments. In-situ observations of dynamo processes require certain physical assumptions to calculate gradients from single-point data in the solar wind. Here we study for the first time the kinematic small-scale dynamo in the turbulent magnetosheath. In the kinematic approach the back reaction of the amplified magnetic field to plasma flows is neglected. Small-scale dynamos can generate or amplify magnetic fields at scales comparable to, or smaller than, the characteristic scales of flow gradients in 3D plasma turbulence. The flow gradients are estimated on the basis of in-situ multi-point MMS measurements. Theoretical predictions and numerical simulation results for the turbulent kinematic dynamo are tested. Specifically, the expected stretching of the magnetic field by velocity gradients, the effect of compressions and the concurrent occurrence of pressure anisotropy instabilities are investigated. The observations show that the magnetosheath data exhibit the expected turbulent dynamo signatures. Since the increase of magnetic field is associated with the loss of kinetic energy, the small-scale dynamo represents an inherent ingredient of plasma turbulence.

How to cite: Vörös, Z., Roberts, O. W., Narita, Y., Emiliya, Y., Nakamura, R., Schmid, D., Settino, A., Wolwerk, M., Wedlund, C. S., Varsani, A., Sorriso-Valvo, L., Bourdin, P. A., and Kis, Á.: Turbulent small-scale kinematic dynamo in the terrestrial magnetosheath, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3759, https://doi.org/10.5194/egusphere-egu25-3759, 2025.

EGU25-4040 | Orals | ST1.11

What determines the departure from equipartition of energy in Alfvénic fluctuations in solar wind streams? Insights from Solar Orbiter observations 

Raffaella D Amicis, Simone Benella, Roberto Bruno, Rossana De Marco, Marco Velli, Denise Perrone, Luca Sorriso Valvo, Benjamin L. Alterman, Nikos Sioulas, Luca Franci, Andrea Verdini, Lorenzo Matteini, Daniele Telloni, Christopher J. Owen, Philippe Louarn, and Stefano Livi

The very first observations by Mariner 5 highlighted the presence of Alfvénic fluctuations in the solar wind identified as nearly incompressible fluctuations accompanied by large correlations between velocity and magnetic field components as predicted by the magnetohydrodynamics (MHD) theory. Since then, Alfvénic fluctuations have been observed to be ubiquitous especially in high-speed solar wind streams, but are also in some cases in slow wind streams, which may in turn exhibit a strong Alfvénic character. The so-called Alfvénic slow wind resembles the fast wind in many aspects, but may also differ from it. Indeed, recent observations performed by Solar Orbiter have shown that the fast wind may display a strong Alfvénic content of the fluctuations than the one observed in the Alfvénic slow wind, especially closer to the Sun.

In this context, Solar Orbiter offers a unique opportunity to study the origin and radial evolution of the Alfvénic solar wind. In this particular study, we present a comparative study between different Alfvénic streams, both fast and slow, at different heliocentric distances, focusing on the characterization of Alfvénicity of different streams with particular reference to the energy balance of the fluctuations.

The aim of this work is to deepen our understanding of what are the mechanisms responsible for the evolution of Alfvénicity in solar wind fluctuations and to understand better to what extent the two solar wind regimes show different Alfvénic content of the fluctuations and eventually evolve in a different way.

How to cite: D Amicis, R., Benella, S., Bruno, R., De Marco, R., Velli, M., Perrone, D., Sorriso Valvo, L., Alterman, B. L., Sioulas, N., Franci, L., Verdini, A., Matteini, L., Telloni, D., Owen, C. J., Louarn, P., and Livi, S.: What determines the departure from equipartition of energy in Alfvénic fluctuations in solar wind streams? Insights from Solar Orbiter observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4040, https://doi.org/10.5194/egusphere-egu25-4040, 2025.

EGU25-4534 | ECS | Orals | ST1.11

Measuring the turbulent energy cascade rate with multiple spacecraft 

Francesco Pecora, Sergio Servidio, Antonella Greco, Yan Yang, William H. Matthaeus, Alexandros Chasapis, Leonardo Primavera, Petr Hellinger, Francesco Pucci, Sean Oughton, David J. Gershman, Barbara L. Giles, and James L. Burch

Exploration of space plasmas is entering a new era of multi-satellite constellation measurements that will determine fundamental properties of turbulence, with unprecedented precision. Familiar but imprecise approximations must be abandoned and replaced with more advanced approaches. We present the novel multispacecraft technique LPDE (Lag-Polyhedra Derivative Ensemble) for evaluating third-order statistics, using simultaneous measurements at many points. The method differs from existing approaches in that (i) it is inherently three-dimensional; (ii) it provides a statistically significant number of estimates from a single data stream; and (iii) it allows for a direct visualization of energy flux in turbulent plasma. Implications for HelioSwarm and Plasma Observatory and comparison with single-spacecraft approaches are discussed.

How to cite: Pecora, F., Servidio, S., Greco, A., Yang, Y., Matthaeus, W. H., Chasapis, A., Primavera, L., Hellinger, P., Pucci, F., Oughton, S., Gershman, D. J., Giles, B. L., and Burch, J. L.: Measuring the turbulent energy cascade rate with multiple spacecraft, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4534, https://doi.org/10.5194/egusphere-egu25-4534, 2025.

EGU25-4798 | Posters on site | ST1.11

Flattening of the magnetic field power spectral density profile 

Jana Safrankova, Zdenek Nemecek, and Frantisek Nemec

The power spectral densities (PSDs) of ion moments and magnetic field turbulence in the solar wind can be fitted by a power law with the power index of -5/3 in the MHD range of frequencies and with the power index ranging from 2 to 4 at frequencies exceeding the proton gyroscale.  However, the density PSD often exhibits a significant flattening at the high-frequency part of the MHD range but a similar effect was not observed for any other quantity. For this reason, the paper analyzes the power spectra of solar wind and magnetic field fluctuations computed in the frequency range around the break between MHD and kinetic scales. We use Spektr-R proton moments and Wind magnetic field at 1 AU and concentrate on the overall PSD profiles of the density, thermal speed, parallel and perpendicular components of magnetic field and velocity fluctuations and investigate statistically the role of parameters like the fluctuation amplitude, collisional age, temperature anisotropy or ion beta. The statistics based on more than 10 thousand of 20-minute intervals shows that the compressive component of magnetic field fluctuations behaves like the density fluctuation in the old, low-beta solar wind. On the other hand, a similar profile was not observed for either bulk or thermal speeds. The dependence on the collisional age initiated the comparison with Solar Orbiter and PSP observations in the inner heliosphere that would shed light on the processes leading to a formation of these spectral features.

How to cite: Safrankova, J., Nemecek, Z., and Nemec, F.: Flattening of the magnetic field power spectral density profile, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4798, https://doi.org/10.5194/egusphere-egu25-4798, 2025.

EGU25-5936 | Posters on site | ST1.11

Rugged magnetohydrodynamic invariants in weakly collisional plasma turbulence 

Petr Hellinger and Victor Montagud Camps

We investigate properties of ideal second-order magneto-hydrodynamic (MHD) and Hall MHD invariants  (kinetic+magnetic energy and different helicities) in a two-dimensional hybrid simulation of decaying plasma turbulence. The combined (kinetic+magnetic) energy decays at large scales, cascades (from large to small scales) via the MHD non-linearity at intermediate scales. This cascade partly continues via the Hall coupling to sub-ion scales. The cascading energy is transferred (dissipated) to the internal energy at small scales via the resistive  dissipation and the pressure-strain effect. The mixed (X) helicity, an ideal invariant of Hall MHD, exhibits a strange behaviour whereas the cross helicity (the ideal invariant in MHD but not in Hall MHD), in analogy to the energy, decays at large scales, cascades from large to small scales via the MHD+Hall non-linearities, and is dissipated at small scales via the resistive dissipation and an equivalent of the pressure-strain effect. In contrast, the magnetic helicity is very weakly generated through the resistive term and does not exhibit any cascade; furthermore, the magnetic and cross helicities are not coupled in the hybrid approximation, so that the corresponding helicity barrier does not exist.

How to cite: Hellinger, P. and Montagud Camps, V.: Rugged magnetohydrodynamic invariants in weakly collisional plasma turbulence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5936, https://doi.org/10.5194/egusphere-egu25-5936, 2025.

EGU25-6875 | Posters on site | ST1.11

Autocorrelation and Cross-Correlation of MHD Turbulence across IP Shock: Multispacecraft Analysis 

Ilyas Abushzada, Alexander Pitna, Zdenek Nemecek, and Jana Safrankova

Turbulent processes play a key role in the dynamics of solar wind plasma fluctuations, governing energy transfer within the heliosphere and driving particle acceleration. In this study, we aim to investigate the nature of large- and small-scale fluctuations in the upstream and downstream regions of interplanetary shocks. By analyzing magnetic field fluctuations using both traditional and recently developed methods, we examine changes in correlation length, Taylor scale, and Reynolds number from upstream to downstream regions. Plasma and magnetic field measurements from the ACE, WIND, and DSCOVR missions are utilized in this analysis. Correlation lengths are determined using autocorrelation and cross-correlation functions applied across data from the three spacecraft. When analyzing the Reynolds number, we observe a decrease in values when transitioning from upstream to downstream regions, suggesting turbulence resetting in the case under consideration. Building on the findings of a case study, we extend our investigation by performing a statistical analysis of these parameters across multiple shocks.

How to cite: Abushzada, I., Pitna, A., Nemecek, Z., and Safrankova, J.: Autocorrelation and Cross-Correlation of MHD Turbulence across IP Shock: Multispacecraft Analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6875, https://doi.org/10.5194/egusphere-egu25-6875, 2025.

The evolving subset of turbulent structures facilitates the energy transfer from large to small spatial scales, on average. Currently, it is not known how the discontinuities that develop between these structures alter the energy transfer in the solar wind. Quantifying the energy transfer to small scales is essential to explain the apparent plasma heating during its advection through the heliosphere. We analyse the energy transfer rate conditioned on the magnetic field line topology of the associated structures in the solar wind. Magnetic field line topology is classified using invariants of the magnetic field gradient tensor constructed from the Cluster spacecraft configuration on scale of approximately 40 proton gyro-radii. Third order structure functions are estimated for five solar wind intervals and conditioned on the contemporaneous values of the topological invariants. We determine how the global mean energy transfer rates correlate with the topology of the turbulence.

How to cite: Hnat, B., Chapman, S., and Watkins, N.: Statistics of the turbulent energy transfer rate conditioned on magnetic field line topology in the solar wind, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6877, https://doi.org/10.5194/egusphere-egu25-6877, 2025.

EGU25-7618 | ECS | Posters on site | ST1.11

Multi-scale Dynamics of Coherent Electron Trapping and Diffusion in Earth's Magnetosheath 

Wence Jiang, Hui Li, Daniel Verscharen, Jiangshan Zheng, Kristopher Klein, Mario Riquelme, Jingting Liu, and Chi Wang
Space and astrophysical plasmas exhibit electromagnetic fluctuations and inhomogeneous structures across a wide range of scales. In the turbulent magnetosheath, high-frequency whistler waves are closely associated with large-scale coherent structures such as magnetic holes. Our study presents statistical evidence on the generation and diffusion efficiency of two distinct groups of whistler modes. Temperature-anisotropy and beam-type instabilities are triggered at different stages of magnetic hole evolution. We introduce a quasi-linear model demonstrating the crucial role of adiabatic trapping and cooling of electrons in generating these whistler waves. As the magnetic hole steepens, the slow evolution of unstable electron velocity distribution functions indicates a transition from temperature-anisotropy to beam-type instabilities, which reach saturation at faster time scales. This multi-scale mechanism offers new insights into the excitation and dissipation of whistler-mode fluctuations in similar environments.

How to cite: Jiang, W., Li, H., Verscharen, D., Zheng, J., Klein, K., Riquelme, M., Liu, J., and Wang, C.: Multi-scale Dynamics of Coherent Electron Trapping and Diffusion in Earth's Magnetosheath, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7618, https://doi.org/10.5194/egusphere-egu25-7618, 2025.

EGU25-9622 | Orals | ST1.11

Decay of magnetohydrodynamic turbulence in the expanding solar wind: WIND observations 

Andrea Verdini, Petr Hellinger, Simone Landi, Roland Grappin, Victor Montagud-Camps, and Emanuele Papini

We have studied the decay of turbulence in the solar wind. Fluctuations carried by the expanding wind are naturally damped because of flux conservation, slowing down the development of a turbulent cascade. The latter also damps fluctuations but results in plasma heating. We analyzed time series of the velocity and magnetic field (v and B, respectively) obtained by the WIND spacecraft at 1 au. Fluctuations were recast in terms of the Elsasser variables, z± = v ± B/√4πρ, with ρ being the average density, and their second- and third-order structure functions were used to evaluate the Politano-Pouquet relation, modified to account for the effect of expansion.

We find that expansion plays a major role in the Alfvénic stream, those for which z+ ≫ z‑. In such a stream, expansion damping and turbulence damping act, respectively, on large and small scales for z+, and also balance each other. Instead, z‑ is only subject to a weak turbulent damping because expansion is a negligible loss at large scales and a weak source at inertial range scales.

These properties are in qualitative agreement with the observed evolution of energy spectra that is described by a double power law separated by a break that sweeps toward lower frequencies for increasing heliocentric distances. However, the data at 1 au indicate that injection by sweeping is not enough to sustain the turbulent cascade. We derived approximate decay laws of energy with distance that suggest possible solutions for the inconsistency: in our analysis, we either overestimated the cascade of z± or missed an additional injection mechanism; for example, velocity shear among streams.

How to cite: Verdini, A., Hellinger, P., Landi, S., Grappin, R., Montagud-Camps, V., and Papini, E.: Decay of magnetohydrodynamic turbulence in the expanding solar wind: WIND observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9622, https://doi.org/10.5194/egusphere-egu25-9622, 2025.

EGU25-9809 | Posters on site | ST1.11

Evolution of Turbulent Fluctuations across Terrestrial Bow Shock 

Alexander Pitna, Gary Zank, Lingling Zhao, Masaru Nakanotani, Sujan Prasad Gautam, Ashok Silwal, Ilyas Abushzada, Byeongseon Park, Jana Safrankova, and Zdenek Nemecek

Magnetohydrodynamic (MHD) shocks are one of the key nonlinear phenomena which occur in plasmas and can influence a dynamical evolution of a system at wide range of spatial scales. In the vicinity of the shock fronts, a majority of the dissipation of the incident bulk energy takes place. Furthermore, the incident fluctuations have profound effect on the shock front itself and also on the respective evolution of the transmitted/generated modes. Recently, several approaches have been developed focusing on the evolution of various plasma wave modes across MHD shocks. In this work, we investigate the transmission of quasi-2D turbulent fluctuations across fast forward shocks in the framework of the Zank et al. (2021) model. We take advantage of concurrent measurements of upstream and downstream plasma of a terrestrial bow shock, employing observations of the Wind spacecraft and Magnetophere Multiscale Mission (MMS). This partially mitigates two main limitations of single spacecraft studies, (a) the variability of incident plasma and magnetic field fluctuations and (b) the effects that stem from the evolution of fluctuations as they propagate away from the shock front. Our results suggest that the Zank et al. (2021) model predicts the downstream levels of fluctuations excellently for the quasi-perpendicular regime of the bow shock. We discuss the deviations between the predicted and observed levels of downstream fluctuations, highlighting the influence of bow shock nonplanarity and variable obliquity.

How to cite: Pitna, A., Zank, G., Zhao, L., Nakanotani, M., Gautam, S. P., Silwal, A., Abushzada, I., Park, B., Safrankova, J., and Nemecek, Z.: Evolution of Turbulent Fluctuations across Terrestrial Bow Shock, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9809, https://doi.org/10.5194/egusphere-egu25-9809, 2025.

EGU25-10420 | Posters on site | ST1.11

Evolution of Turbulent Energy Dissipation at Quasi-perpendicular Fast Interplanetary Shocks: The thickness of shock transition region 

Byeongseon Park, Alexander Pitna, Jana Safrankova, and Zdenek Nemecek

We present a comprehensive analysis of the evolution of the turbulent energy dissipation at interplanetary (IP) shocks observed by Parker Solar Probe (≈0.4 AU), Solar Orbiter (≈0.8 AU), and Wind (1 AU). Our previous study reveals the conservation of the energy dissipating mechanisms across different types of IP shocks except fast reverse. Motivated to investigate the thickness of the shock transition region in terms of the dissipation of magnetic field turbulent energy, we adopt pairs of quasi-perpendicular fast forward (FF) and reverse (FR) shocks observed at Parker Solar Probe, Solar Orbiter, and Wind. By comparing these pairs of shock, we anticipate examining (1) whether FF and FR shocks are systematically different, (2) the dependence of the shock transition thickness on critical Mach number, and (3) on heliocentric distance. We present several parameters, i.e., cross- and magnetic helicity, and the amplitude of magnetic field fluctuations for the estimation of their correlation with the spectral index evolving through shock. The abrupt changes of the plasma parameters along with the spectral index shorter than the temporal resolution of the plasma measurement are overall observed showing their minimal correlations. This suggests a role of IP shock as a thin boundary simply distinguishing two different plasmas. We will extend this hypothesis toward a statistical study including near-shock processes such as particle acceleration and wave activities.

How to cite: Park, B., Pitna, A., Safrankova, J., and Nemecek, Z.: Evolution of Turbulent Energy Dissipation at Quasi-perpendicular Fast Interplanetary Shocks: The thickness of shock transition region, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10420, https://doi.org/10.5194/egusphere-egu25-10420, 2025.

EGU25-11551 | Posters on site | ST1.11

Emergence of a characteristic scale in the Alfvénic solar wind turbulence 

Luca Sorriso-Valvo, Shiladittya Mondal, Supratik Banerjee, Andrea Larosa, Honghong Wu, Nikos Sioulas, Daniele Telloni, Raffaella D'Amicis, and Emiliya Yordanova

The solar wind is highly turbulent, which results in power-law spectra and intermittency for magnetic and velocity fluctuations within the inertial range. 
Using fast solar wind intervals measured during solar minima between 0.3 au and 3.16 au, a clear break emerges within the traditional inertial range, with signatures of two inertial sub-ranges with f-3/2 and f-5/3 power laws in the magnetic power spectra. The intermittency, measured through the scaling law of the kurtosis of magnetic field fluctuations, further confirms the existence of two different power laws separated by a clear break. A systematic study on the evolution of the said sub-ranges as a function of heliospheric distance shows correlation of the break scale with both the turbulence outer scale and the typical ion scales. Finally, using Parker Solar Probe data measured closer to the Sun, we highlight the role of switchbacks and switchback patches in generating such scale breaks.

How to cite: Sorriso-Valvo, L., Mondal, S., Banerjee, S., Larosa, A., Wu, H., Sioulas, N., Telloni, D., D'Amicis, R., and Yordanova, E.: Emergence of a characteristic scale in the Alfvénic solar wind turbulence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11551, https://doi.org/10.5194/egusphere-egu25-11551, 2025.

EGU25-11571 | Posters on site | ST1.11

Solar wind turbulent fluctuations within the kinetic range of scales 

Olga Alexandrova, Dusan Jovanovic, Petr Hellinger, Pascal Demoulin, Milan Maksimovic, Stuart Bale, and Andre Mangeney

Electromagnetic fluctuations in the solar wind cover a wide range of scales, from sun-rotation period to sub-electron scales. We study Cluster Guest Investigator data when 2 satellites were at 7 km distance, that corresponds to few electron Larmor radius. We find a typical spectral shape within the kinetic range and signatures of intermittency up to electron scales. Local analysis of magnetic fluctuations at electron scales indicates presence of vortex-like coherent structures, which can be interpreted in terms of electron scale Alfven vortices. We discuss a possible connection of these small-scale vortices with coherent structures at ion scales. The results at 1 au will be compared with spectral properties and coherent structures at kinetic scales observed by Parker Solar Probe closer to the Sun.

How to cite: Alexandrova, O., Jovanovic, D., Hellinger, P., Demoulin, P., Maksimovic, M., Bale, S., and Mangeney, A.: Solar wind turbulent fluctuations within the kinetic range of scales, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11571, https://doi.org/10.5194/egusphere-egu25-11571, 2025.

In the transition range of the solar wind turbulence, the magnetic spectrum has been observed to be strongly anisotropic with respect to local mean field. However, the generation mechanism of the anisotropy remains not well understood. There are two typical types of waves existing in the transition range, including ion cyclotron waves (ICWs) and kinetic Alfven waves (KAWs) propagating in the directions parallel and perpendicular to magnetic field, respectively. In this work, we perform a statistical study on the effects of the waves on the spectral anisotropy of the transition range. We select 31 intervals from the measurements of Parker Solar Probe between 2018 and 2021. The magnetic helicity (sigma_m) diagnosis is applied on the magnetic field data at the frequency domain [0.1 Hz, 10 Hz], and the wavelet coefficients with sigma_m < -0.5 and sigma_m > 0.4 are considered as signals of ICWs and KAWs, respectively. We then remove them and find that the spectral anisotropy in the transition range becomes significantly weaker. Specifically, the spectra in the quasi-parallel direction statistically get shallower, and the average spectral index changes from -5.68±0.74 to -4.72±0.56. By contrast, the spectra in the perpendicular direction get slightly steeper, and the index changes from -3.63±0.34 to -3.95±0.41. Moreover, the anisotropic scaling in the transition range is found to be k ~ k1.55±0.33. The new results about the magnetic field spectra after the removal of ICW and KAW will help to further understand the possible mechanisms that cause the spectral anisotropy in the transition range.

How to cite: Wang, X. and Zhang, H.: Effects of Waves on the Spectral Anisotropy of Transition Range in the Solar Wind Turbulence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14164, https://doi.org/10.5194/egusphere-egu25-14164, 2025.

EGU25-14248 | Posters on site | ST1.11

Identifying Kinetic Phase Space Signatures of Turbulent Dissipation 

Trevor Bowen, Tamar Ervin, Alexandros Chasapis, Oreste Pezzi, Andrea Larosa, Kris Klein, Alfred Mallet, and Stuart Bale

Understanding the nature and importance of various proposed heating processes that result from turbulent dissipation is imperative in describing a range of collisionless systems. We highlight the importance of kinetic phase space signatures of heating as pivitol in providing necessary contraints on turbulent dissipation. Understanding mechanisms through diffusive approximation schemes is largely a tractable problem that can be studied with modern plasma instrumentation. We highlight recent progress in understanding signatures of kinetic dissipation and particle heating using the Parker Solar Probe (PSP) mission. Importantly, our observations reveal that a range of heating mechanisms (stochastic heating, cyclotron resonance, and Landau damping) are likely important in explaining observed phase-space plasma signatures. The use of non-parametric approximations to particle distribution functions (via Hermite polynomials and Radial Basis Functions) is pivotal in understanding and characterizing these heating mechanisms. While our observations are from PSP, we discuss furture implementation of these techniques on current and future plasma missions (MMS and Plasma Observatory).

How to cite: Bowen, T., Ervin, T., Chasapis, A., Pezzi, O., Larosa, A., Klein, K., Mallet, A., and Bale, S.: Identifying Kinetic Phase Space Signatures of Turbulent Dissipation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14248, https://doi.org/10.5194/egusphere-egu25-14248, 2025.

EGU25-14782 | Orals | ST1.11

A new scenario with two subranges in the inertial regime of solar wind turbulence 

Honghong Wu, Shiyong Huang, Jiansen He, Liping Yang, Luca Sorriso-Valvo, Xin Wang, and Zhigang Yuan

Solar wind provides a natural laboratory for the plasma turbulence. The core problem is the energy cascade process in the inertial range, which has been a long-standing fundamental question. Many efforts are put into the theoretical modellings to explain the observational features in the solar wind. However, there are always questions remained. Here we report a new scenario that the inertial regime of the solar wind turbulence consists of two subranges based on the observation. We perform multi-order structure function analyses for one high-latitude fast solar wind interval at 1.48 au measured by Ulysses and one slow solar wind at 0.17 au measured by Parker Solar Probe (PSP). We identify the existence of two subranges in the inertial range according to their distinct scaling features. Based on the observational features, we propose that the possible mechanisms that subrange 1 is Iroshnikov-Kraichnan-like turbulence and subrange 2 is the intermittency-dominated region. The scenario of two subranges and their scaling laws not only shed new lights for the plasma turbulence, but also unify previous results that cause debates, making the observed scaling laws prepared for further theoretical modeling. 

How to cite: Wu, H., Huang, S., He, J., Yang, L., Sorriso-Valvo, L., Wang, X., and Yuan, Z.: A new scenario with two subranges in the inertial regime of solar wind turbulence, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14782, https://doi.org/10.5194/egusphere-egu25-14782, 2025.

EGU25-15511 | ECS | Posters on site | ST1.11

Turbulence features of the solar wind from different source regions based on Parker Solar Probe observation 

Tieyan Wang, Wenhao Chen, Liping Yang, Jiansen He, and Hui Fu

Properties of the solar wind in different types of plasma (e.g., heliospheric current sheet, coronal hole, ejecta, sub-Alfvénic) are known to exhibit distinct features. Based on Parker Solar Probe measurements of the solar wind in the inner heliosphere, we compare the similarities and differences between two streams originating from different sources at the same radial distance. Despite sharing similar properties, including cross helicity, residual energy, Elsasser ratio, and magnetic compressibility, notable differences are observed. For the solar wind associated with active regions, the turbulence exhibits lower magnetic field fluctuation amplitudes, shallower magnetic field spectrum, and stronger intermittency, whereas the turbulence associated with coronal holes displays opposite characteristics. The switchback properties of these two streams are also discussed. Our results further explore the variabilities of solar wind turbulence, which may have implications for solar wind heating and acceleration.

How to cite: Wang, T., Chen, W., Yang, L., He, J., and Fu, H.: Turbulence features of the solar wind from different source regions based on Parker Solar Probe observation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15511, https://doi.org/10.5194/egusphere-egu25-15511, 2025.

EGU25-16301 | ECS | Posters on site | ST1.11

Third-Order Law for MHD Turbulence Varying the Dissipation Mechanisms 

Elisa Maria Fortugno, Luisa Scarivaglione, Sergio Servidio, and Vincenzo Carbone

The phenomenon of energy cascade in Alfvénic solar wind turbulence has traditionally been studied assuming ideal plasmas, where viscosity (ν) and resistivity (η) are equal and very small. However, recent observations suggest that in the solar wind, viscous-like effects related to velocity act on much larger scales compared to magnetic dissipation. The main novelty of this study lies in assuming phenomenological distinctions among dissipation mechanisms and hence assuming different values for ν and η.

In this work, we investigate the third-order Yaglom law for magnetohydrodynamic (MHD) turbulence through a combination of theoretical analysis and simulations. Specifically, we study the energy budget law for visco-resistive MHD and explore how differing viscosities and resistivities affect the energy cascade. The Yaglom relation, rewritten in terms of Elsässer variables, deviates from the ideal case due to the assumption ν ≠ η. This relation, which involves a third-order moment calculated from velocity and magnetic fields, provides a direct measure of the energy transfer rate across scales.

Our preliminary results, supported by direct numerical simulations, indicate that these findings could enhance the interpretation of solar wind and magnetosheath observations. The third-order moment is indeed particularly relevant as it enables a detailed comparison of energy transfer mechanisms, highlighting the differences that arise when the dissipation processes in the velocity and the magnetic field are different.

How to cite: Fortugno, E. M., Scarivaglione, L., Servidio, S., and Carbone, V.: Third-Order Law for MHD Turbulence Varying the Dissipation Mechanisms, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16301, https://doi.org/10.5194/egusphere-egu25-16301, 2025.

EGU25-17216 | ECS | Posters on site | ST1.11

A mass invariant in a compressible turbulent medium 

Pierre Dumond, Jérémy Fensch, Gilles Chabrier, and Etienne Jaupart

Turbulence is ubiquitous in star-forming regions, but predicting measurable statistical properties of the density fluctuations in a supersonic compressible turbulent flow is a major challenge in physics. In 1951, Chandrasekhar derived an invariant Minv under the assumption of the statistical homogeneity and isotropy of the turbulent density field and stationarity of the background density. Recently, Jaupart & Chabrier (2021) extended this invariant to non-isotropic flows in a time-evolving background and showed that it has the dimension of a mass. This invariant depends on the variance and correlation length of the density field. In this work, we perform numerical simulations of homogeneous and isotropic compressible turbulence to test the validity of this invariant in a medium subject to decaying turbulence or to self-gravity. We study several input configurations, namely different Mach numbers, injection lengths of turbulence, equations of state and average gas densities to cover the variety of star formation conditions. We confirm that Minv remains constant during the decaying phase of turbulence and also when for self-gravitating flows. Furthermore, we develop a theoretical model of the density field statistics which predicts without any free parameters the evolution of the correlation length with the variance of the logdensity field beyond the assumption of the gaussian field for the logdensity. Noting that Minv is independent of the Mach number, we show that this invariant can be used to relate the non-gaussian evolution of the logdensity probability distribution function to its variance with no free parameters. Finally, we will discuss what we can learn from this invariant in terms of the statistics of the structures formed in star-forming regions.

How to cite: Dumond, P., Fensch, J., Chabrier, G., and Jaupart, E.: A mass invariant in a compressible turbulent medium, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17216, https://doi.org/10.5194/egusphere-egu25-17216, 2025.

EGU25-17439 | ECS | Posters on site | ST1.11

Small-scale Current Sheets and Magnetic Reconnection in the Turbulent Solar Wind 

Inmaculada F. Albert, Sergio Toledo-Redondo, Víctor Montagud-Camps, Aida Castilla, Benoît Lavraud, Naïs Fargette, Philippe Louarn, Christopher Owen, and Yannis Zouganelis

Magnetic reconnection is an energy dissipating process, in which magnetic field topology is modified, eroding the magnetic field, and turning the magnetic energy into thermal and kinetic energy of the plasma. Magnetic reconnection has been observed through a wide range of scales in the solar system, from thousands of ion inertial lengths in the heliospheric current sheet to few electron inertial lengths in Earth’s magnetosheath. However, the smaller scales were not accessible in the solar wind until the launch of Solar Orbiter and Parker Solar Probe, and therefore ion-scale magnetic reconnection had not been studied in the solar wind.

 

Non-linear interactions drive turbulence in the solar wind, transferring energy across scales at a constant rate, seen as a constant slope in the energy spectrum of magnetic fluctuations. However, a spectral break is observed at scales close to and below the ion inertial length. It has been proposed that the magnetic energy dissipated through magnetic reconnection at scales of the ion inertial length or smaller can account in part for this break in the magnetic fluctuation energy spectrum.

 

In the present work, we have harnessed the high cadence of the Solar Orbiter in-situ instrumentation (Solar Wind Analyzer and Magnetometer) to search for magnetic reconnection at scales in the order of few to tens ion inertial lengths. We compiled a catalog of 979 thin current sheets, 5% of which undergo reconnection. Statistics of CS properties and Solar Wind conditions around these has been performed, with a double aim: assessing the relation between turbulence and reconnection; and evaluate the influence of different Solar Wind parameters on ion-scale reconnection.

How to cite: F. Albert, I., Toledo-Redondo, S., Montagud-Camps, V., Castilla, A., Lavraud, B., Fargette, N., Louarn, P., Owen, C., and Zouganelis, Y.: Small-scale Current Sheets and Magnetic Reconnection in the Turbulent Solar Wind, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17439, https://doi.org/10.5194/egusphere-egu25-17439, 2025.

EGU25-17532 | Orals | ST1.11

On the velocity phase space cascade in the inner heliosphere 

Andrea Larosa, Oreste Pezzi, Trevor Bowen, Alexandros Chasapis, Domenico Trotta, Luca Sorriso-Valvo, Christopher Chen, Roberto Livi, and Jaye Verniero

In space plasma, due to the absence of collisions, the phase space present a complex structuring and strong deviations from thermal equilibrium. Previous works have highlighted this aspect in both magnetosheath data and numerical simulation through an hermite decomposition of the ion velocity distribution function. The hermite spectrum of the vdf is expected to to have a precise spectral slope and to present anisotropy in a magnetic field dominated environment. Such a tool is particularly suited for the vdf representation since each order of the hermite decomposition corresponds to a moment of the vdf.

In this work we study, by using the Parker Solar Probe ion vdfs, the evolution of the hermite spectrum and the vdf fine features with respect to radial distance and solar wind conditions.

These results are useful to understand how the phase space evolve in the inner heliosphere and how this effect the heating in collissionless plasma.

How to cite: Larosa, A., Pezzi, O., Bowen, T., Chasapis, A., Trotta, D., Sorriso-Valvo, L., Chen, C., Livi, R., and Verniero, J.: On the velocity phase space cascade in the inner heliosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17532, https://doi.org/10.5194/egusphere-egu25-17532, 2025.

EGU25-18278 | ECS | Orals | ST1.11

On the role of mirror mode instabilities in the reconnecting Heliospheric Current Sheet dynamics 

Naïs Fargette, Jonathan Eastwood, Lorenzo Matteini, Cara L. Waters, Vincent Génot, and Victor Réville

Magnetic reconnection is a fundamental process in astrophysical plasma, as it enables the dissipation of energy at kinetic scales as well as large-scale reconfiguration of the magnetic topology. In the solar wind, its quantitative role in plasma dynamics and particle energization remains an open question that is starting to come into focus as more missions now probe the inner heliosphere. In particular, the first encounters of the Parker Solar Probe (PSP) mission with the Sun have revealed that the Heliospheric Current Sheet (HCS) was often reconnecting close to the Sun, opening question about the impact of HCS reconnection on the nearby solar wind.

In this work, we first make a thorough catalog of all HCS crossings measured PSP (encounter 5 to the latest available) and find that 88\% of crossings present magnetic reconnection signatures. This statistically confirms that magnetic reconnection is prevalent in the near Sun HCS. We then quantify the level of turbulence within the HCS and find enhanced energy at kinetic scales compared to the nearby solar wind, usually devoid of magnetic switchbacks. We furthermore highlight the frequent observation of mirror mode instabilities within the structure of the HCS, hinting that this process plays a particular role in the energy dissipation. These mirror mode instabilities are also observed within HCS crossings observed by Solar Orbiter further in the heliosphere. We finally plan to study the evolution of the HCS structure through multi-spacecraft observation.

Collectively, these results show that the HCS may play an important role in the energization of the near Sun solar wind. We discuss the impact of these observations on our current understanding of HCS reconnection and solar wind turbulence.

How to cite: Fargette, N., Eastwood, J., Matteini, L., Waters, C. L., Génot, V., and Réville, V.: On the role of mirror mode instabilities in the reconnecting Heliospheric Current Sheet dynamics, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18278, https://doi.org/10.5194/egusphere-egu25-18278, 2025.

EGU25-205 | ECS | Posters on site | HS1.1.4

Modeling the Ammonium Removal Processes in Household Sand Filters 

Ran Wei, Anh Van Le, Binlong Liu, Mohammad Azari, Wolfgang Nowak, Andreas Kappler, and Sergey Oladyshkin

Elevated ammonium (NH4+) concentrations in groundwater (GW) pose significant challenges to existing GW treatment systems, particularly in simplified systems such as household sand filters (HSFs), which are widely used in developing countries. We previously conducted a series of column experiments (sand filter materials collected in Hanoi, Vietnam) mimicking HSFs. These experiments revealed limited and fluctuating NH4+ removal, highlighting the need for a comprehensive process-based model to elucidate the complex interplay of physical and biochemical processes that influence NH4+ concentration dynamics in these systems. Here, we established a one-dimensional advective-dispersive-reactive model conditioned on data from column experiments under laboratory (artificial GW inflow with sand materials from local HSFs) and field conditions (natural GW inflow with sand materials from local supplier), accounting for temporal variations in reaction kinetics, transport processes, and a previously unconsidered inter-phase transfer process for nitrate (NO3-). The modeled breakthrough curves capture the complex dynamics of NH4+, nitrite (NO2-), and NO3- concentrations under both laboratory and field conditions. The reaction rates of the nitrogen species show strong hysteresis in response to substrate (NH4+ and NO2-) concentrations, suggesting that potential lags in the biochemical reactions caused by inhibitions and low retention time lead to the incomplete NH4+ removal. Our scenario analysis indicates that, without inhibition effects, the current bio-reactive environment could reduce NH4+ concentrations to the legal target level (within up to eight hours retention time under field conditions). This study represents one of the few process-based modeling efforts mimicking HSFs. Future modeling research should parameterize various inhibition effects into the existing reactive transport models in order to gain quantitative insight into enhancement methods for HSFs.

How to cite: Wei, R., Le, A. V., Liu, B., Azari, M., Nowak, W., Kappler, A., and Oladyshkin, S.: Modeling the Ammonium Removal Processes in Household Sand Filters, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-205, https://doi.org/10.5194/egusphere-egu25-205, 2025.

Abstract

Arsenic (As) contamination in groundwater is a serious environmental and public health issue, particularly in regions where groundwater is a primary source of drinking water. Many Asian countries, particularly Bangladesh, India and parts of Southeast Asia are adversely affected with As contaminated aquifers. The present study thus aims to explore the source, distribution and release mechanism of As into the groundwater in the parts of southern bank of the Upper Brahmaputra floodplains in Assam, India.  Groundwater samples (n=100) were collected from the shallow aquifers (< 30 m) from two the districts Jorhat and Golaghat, and were analysed for major ions (Ca2+, Na+, K+, Mg2+, Cl-,HCO3-, NO3-,SO42-) and trace elements (As, Fe, Mn, Pb, Co, Cu, Zn). Concentration of As, Fe and Mn in the aquifers has exceeded the permissible limits set by WHO (World Health Organisation) posing serious threat to human health. 54% of groundwater samples have exceeded WHO permissible limit of 10 µg/L for As (range: bdl (below detection limit) to 480 µg/L, mean: 31µg/L). While 94% (range: 0.076 mg/L to 41.37 mg/L, mean: 10.92) and 77% (range: 0.002 mg/L to 9.06 mg/L, mean: 0.6 mg/L) of groundwater samples have exceeded the WHO permissible limit of 0.3 mg/L and 0.05 mg/L for Fe and Mn respectively. Aquifers enriched with As was found adjacent to Naga foothills while low As was found near the Brahmaputra river. Aquifer lithology reveals the presence of thick clay layer near the Naga hills (also indicated by higher Al2O3 in the sediments) and subsequently minerals like illite and kaolinite was found in these clay layers (confirmed by the XRD peaks). The clay minerals might have acted as the active site for adsorption of As, thus acting as the host for As in the studied region. Moreover, the average value (mean: 80) of Chemical Index of alteration (CIA) indicates intense chemical weathering at the source area in warm and humid condition leading to formation of copious amount of clay minerals like kaolinite. No strong co relation was seen between As and the redox sensitive elements viz; Fe and Mn, nor with HCO3, NO3 or SO4 indicating multitudinous processes or reactions viz competitive exchange with anion, reductive dissolution and pH dependent sorption might have control the release of As in the studied region. Higher LREE compared to HREE indicates the source of these clastic sediments could be from felsic or intermediate composition of rocks. Principle Component Analysis (PCA) and cluster analysis indicated the dominance of geogenic factors as the main contribution of these contaminants in the groundwater of the study area. Regular monitoring and intervention of groundwater in the region is crucial for its prolong use. The present study will assist stakeholders and policy maker in taking evidence-based decision and providing As safe drinking water to the affected communities

Key words: Arsenic; Groundwater; Brahmaputra floodplains; Sediment Geochemistry; Hydrochemistry

How to cite: Medhi, S. and Choudhury, R.: Arsenic toxicity in Groundwater of Brahmaputra Floodplains of Assam, India: Concerns for drinking water quality, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1106, https://doi.org/10.5194/egusphere-egu25-1106, 2025.

EGU25-3798 | ECS | Posters on site | HS1.1.4

Selecting an Appropriate Surrogate for Assessing Filtration Removal of Cryptosporidium parvum for Water Treatment Applications 

Margaret E. Stevenson, Liping Pang, Andreas H. Farnleitner, Gerhard Lindner, Alexander K.T. Kirschner, Alfred P. Blaschke, and Regina Sommer

Cryptosporidium parvum is a pathogen causing gastrointestinal infections, occasionally leading to death in immunocompromised individuals. It can contaminate surface water and groundwater, and consequently drinking water supplies, through agricultural activities such as cattle and dairy farming or the spreading of manure as fertilizer. The importance of removing C. parvum by filtration is of great interest because of its long-term persistence in water as oocysts and its resistance to chemical disinfection owing to its thick cell wall. This is relevant for both subsurface filtration and engineered filtration processes. Therefore, it is necessary to evaluate its removal efficiency in subsurface media and during the filtration stage of drinking water treatment. This study aimed to select an appropriate surrogate for C. parvum oocysts that exhibits similar attenuation and transport behaviour through porous media, is cost-effective, and poses no harm to humans or the environment, enabling its application in engineered installations and field studies.

Bacillus subtilis is commonly used as a conservative surrogate for C. parvum for subsurface transport studies, and aerobic spores have been included by the U.S. Environmental Protection Agency as an indicator for C. parvum in groundwater under the direct influence (GWUDI) of surface water. While B. subtilis may be a cost-effective option, its smaller size (nearly 6 times smaller in diameter), different shape (rod-shaped vs. spherical), and distinct surface characteristics present limitations. This study evaluated the attenuation and transport of B. subtilis spores, oocyst-sized unmodified (yellow-green and yellow-orange) and glycoprotein-coated microspheres, along with UV inactivated C. parvum in columns packed with silica sand. The objective was to determine the significance of size, surface charge, and macromolecules on the cell wall surface, on the reduction of the oocysts. Glycoprotein-coated microspheres, exhibiting similar physicochemical properties (including macromolecules) to oocysts, were found to be the most effective surrogate. The study results highlight the importance of selecting appropriate surrogates for accurate evaluation of the transport of C. parvum in the subsurface and its removal in water treatment through sand filtration.

How to cite: Stevenson, M. E., Pang, L., Farnleitner, A. H., Lindner, G., Kirschner, A. K. T., Blaschke, A. P., and Sommer, R.: Selecting an Appropriate Surrogate for Assessing Filtration Removal of Cryptosporidium parvum for Water Treatment Applications, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3798, https://doi.org/10.5194/egusphere-egu25-3798, 2025.

EGU25-4185 | ECS | Posters on site | HS1.1.4

Transport of pathogens in saturated porous rocks under variable flow and salinity 

Alessandro Ghirotto, Valentina Prigiobbe, Maria Clementina Caputo, Osvalda De Giglio, Giorgio Cassiani, Mert Çetin Ekiz, Antonietta Celeste Turturro, Antonella Francesca Savino, Debora Colella, Gavin Barboza, Mirco Milani, and Marco Verani

The transport of pathogens through rocks is often regarded as negligible unless there are fractures in the medium. However, sedimentary rocks may have a porosity that allows the migration of pathogens even when they are unfractured.
In this work, we investigated the transport behavior of several pathogens (namely Escherichia coli and Enterococci faecalis) through a sedimentary porous rock made of 98.5 wt.% of calcite (CaCO3), hydraulic conductivity 6·10−6 m/s, and porosity 0.43. Core flooding experiments were performed under variable head conditions, ensuring full saturation of the samples. During the experiments, the flow and pathogen concentration were monitored. After an initial stabilization of the core, a suspension containing a known concentration of pathogens was superimposed onto the sample and allowed to drain through. Upon complete suspension drainage, several cycles of sterile saline solution (0.9 vol.%) were performed until the pathogen concentration at the outlet became negligible. A reactive transport model through saturated porous media was developed and implemented to describe the tests. The model couples conservation laws for flow and transport under variable head conditions with constitutive equations of straining and attachment/detachment. The data show significant retention of pathogens within the core during suspension drainage and rapid mobilization during distilled water infiltration. This behavior is well captured by the model and shows that rocks can act as bioreactors for pathogens that favor accumulation and growth during loading and mobilization during flooding with low-salinity water. This may suggest that porous rock deposits may exacerbate contamination of the underlying aquifers under intermittent conditions of accumulation/growth and release rather than protecting underground water resources, as generally assumed.
This topic is the objective of DY.MI.CR.ON. project “Predictive dynamics of microbiological contamination of groundwater in the earth critical zone and impact on human health (DY.MI.CR.ON Project)” funded by the European Union – Next Generation EU, mission 4 component 1, CUP I53D23000500001.

How to cite: Ghirotto, A., Prigiobbe, V., Caputo, M. C., De Giglio, O., Cassiani, G., Ekiz, M. Ç., Turturro, A. C., Savino, A. F., Colella, D., Barboza, G., Milani, M., and Verani, M.: Transport of pathogens in saturated porous rocks under variable flow and salinity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4185, https://doi.org/10.5194/egusphere-egu25-4185, 2025.

EGU25-7415 | Posters on site | HS1.1.4

Temporal stability of microbial water quality in small  irrigation water sources 

Yakov Pachepsky, Matthew Stocker, Jaclyn Smith, James Widmer, Dana Harriger, Donjin Jeon, Billie Morgan, Seokmin Hong, Andrew van Tassel, Insuck Baek, Laurel Dunn, Alisa Coffin, Oliva Pisani, and Moon Kim

 

Streams and ponds used for local irrigation tend to demonstrate high spatiotemporal variability of water quality. Microbial water quality monitoring becomes overly resource-demanding if the water quality metrics are treated as purely random values. Research on several irrigation ponds and streams showed relatively stable spatial patterns of microbial and other water quality metrics. Detection of those patterns was achieved by setting 20 to 30 monitoring locations, visiting each location seven to ten times during the irrigation season, measuring the water quality metrics at each location with in situ sampling in water samples, computing relative differences between the measurements in each sampling location, computing the average value of those measurements across the water source for each visit, and finally computing the mean relative differences (MRD) for each location over all the visits. Positive MRDs indicated the preponderance of elevated values of water quality variables, and negative MRDs indicated the prevalence of low values. The nearshore locations typically had the largest MRD in ponds, and the locations with more populated stream reaches. 

Unmanned aerial vehicles were used for multispectral imaging of some ponds on each visit to several ponds before the water sampling. Both reflectance and remote sensing indices were determined at the same locations where water quality metrics were measured. The stable temporal patterns were detected for reflectance and remote sensing indices. Strong significant Spearman correlations were found between stable patterns of some water quality variables and remote sensing indices. Those correlations indicate the opportunities to use UAV-based remote sensing of irrigation water sources to inform the design of sampling water across ponds. Correlations between stable patterns of water quality variable patterns may help in developing monitoring design schemas when the more readily available water quality variable patterns are known.

Establishing temporally stable spatial patterns via the mean relative differences points to locations where monitoring locations could be placed to represent the average across the pond or stream. Also, locations with low MRDs of the microbial pollution metrics appeared to be more suitable for establishing the irrigation water intake. Overall, stable water quality patterns, when detected, can provide useful guidance for establishing and monitoring water quality for those water sources.

How to cite: Pachepsky, Y., Stocker, M., Smith, J., Widmer, J., Harriger, D., Jeon, D., Morgan, B., Hong, S., van Tassel, A., Baek, I., Dunn, L., Coffin, A., Pisani, O., and Kim, M.: Temporal stability of microbial water quality in small  irrigation water sources, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7415, https://doi.org/10.5194/egusphere-egu25-7415, 2025.

EGU25-8167 | Posters on site | HS1.1.4

Resilience to Future Changes: Assessing the Impact of Human Wastewater Emissions on Microbiological Water Safety Along the Danube  

Julia Derx, Peter Valent, Sophia Steinbacher, Ahmad Ameen, Anna-Maria König, Katalin Demeter, Rita Linke, Regina Sommer, Gerhard Lindner, Alois W. Schmalwieser, Julia Walochnik, Alexander Kirschner, Robert L. Mach, Sílvia Cervero-Aragó, Matthias Zessner, Steffen Kittlaus, Günter Blöschl, Margaret Stevenson, Alfred Paul Blaschke, and Andreas H. Farnleitner

Transboundary rivers are crucial resources for drinking water, recreation, and irrigation. However, wastewater emissions and global environmental and demographic changes can impair raw water quality and pose risks to public health. This study aims to assess the impact of emissions from wastewater treatment plants, combined sewer overflows (CSOs), and inland waterway transport on microbiological water safety along the upper Danube River Basin (DRB).

To achieve this, we developed a stochastic mathematical model to trace pathogen load emissions throughout the river network. The model predicts concentrations of reference pathogens (Cryptosporidium, Giardia, Campylobacter, norovirus, enterovirus) in the river for current conditions and a future climate scenario represented by a selected CORDEX RCP 8.5 high emission scenario. The study estimates bathing water infection risks and determines the required pathogen logarithmic reduction in raw river water to ensure safe drinking water. The model accounts for exponential pathogen inactivation rates influenced by water temperature, solar ultraviolet radiation, and lake sedimentation (for protozoan cysts/oocysts). High-resolution navigational information based on automated identification system (AIS) data, detailing the number and location of ships, were used to model the impact of inland waterway transport. The data were aggregated into monthly average daily ship volumes across three ship types (cruise, passenger, and freight) along a section of the Danube River. Model validation was conducted using monthly data sets spanning 2–4 years, including cultivation-based standard fecal indicators, human-associated genetic fecal microbial source tracking markers (HF183/BacR287, BacHum), and reference pathogens (Cryptosporidium, Giardia). Additionally, the study investigates whether the crAssphage marker (CPQ_056) serves as a suitable proxy for human viral fecal contamination in water quality modeling, compared to standardized viral indicators such as somatic coliphages. To understand the effects of future changes on water safety, various scenarios and combinations up to the year 2100 are analyzed, including population growth (affecting wastewater emissions), climate change (impacting river discharge and microbial inactivation), advanced wastewater treatment, reduction of CSOs (in line with the recast of the European Urban Wastewater Treatment Directive), and changes in inland navigation and ship wastewater handling.

The findings indicate that tertiary treated municipal wastewater currently has the greatest impact on river water safety. However, if additional disinfection (quaternary treatment) is implemented, other pollution sources, such as ship navigation and CSOs, as well as climate change effects, will play an increasingly significant role in determining microbiological water safety.

How to cite: Derx, J., Valent, P., Steinbacher, S., Ameen, A., König, A.-M., Demeter, K., Linke, R., Sommer, R., Lindner, G., Schmalwieser, A. W., Walochnik, J., Kirschner, A., Mach, R. L., Cervero-Aragó, S., Zessner, M., Kittlaus, S., Blöschl, G., Stevenson, M., Blaschke, A. P., and Farnleitner, A. H.: Resilience to Future Changes: Assessing the Impact of Human Wastewater Emissions on Microbiological Water Safety Along the Danube , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8167, https://doi.org/10.5194/egusphere-egu25-8167, 2025.

EGU25-8224 | Posters on site | HS1.1.4

From the pasture to the water: multiparametric laboratory experiments to determine microbial release from feces 

Rita Linke, Yanhe Zhou, Gerhard Lindner, Nadine Hochenegger, Tamara Borovec, Georg Reischer, Katarina Priselac, Alba Hykollari, Gabrielle Stalder, Regina Sommer, Julia Derx, and Andreas Farnleitner

To ensure the supply of clean water, we need tools to accurately predict where microorganisms of fecal origin come from, how they move in the environment and where they go to. To date, however, there have been few studies that have looked at bacterial overland transport (BOT). The current state of knowledge is mainly based on data from point sources (sewage treatment plants), whereas little is known about diffuse fecal sources from wildlife and livestock. The aim of this study is therefore to investigate the influence of the type of fecal matter (cow and red deer) as well as storage time and conditions (temperature and moisture) on resuspension and re-mobilization of (genetic) fecal indicators and/or pathogens. For this purpose standardized fecal samples from cow and deer were prepared in the laboratory and stored for different lengths of time (0 to 120 days) under diverse climatic conditions reflecting seasons. Fecal samples were then used in shaking experiments in which the samples were covered with water in Erlenmeyer flasks and placed in a shaking incubator. Different rainfall intensities were simulated by different shaking speeds (60 rpm and 85 rpm) and the effect of the rainfall duration was simulated by the duration of shaking (10 min and 60 min). Cultivation-based methods were used to determine fecal indicator organisms (FIB) such as E. coli, enterococci and Clostridium perfringens spores as well as somatic coliphages in the water. A panel of different qPCR-based DNA and/or RNA markers will then be used to determine host-associated genetic markers (qPCR). This multifactorial experimental approach provides the first quantitative estimates of the persistence and mobility of microbial target organisms in standardized fecal pellets from cattle and deer. The chosen multi-parametric and multi-method approach allows 1) comparison of culture-based with qPCR-based results and 2) comparison of RNA vs. DNA targets. NGS (next generation sequencing) data allows to draw conclusions on intestinal microbial persistence and to evaluate whether they reflect the mobilized load, an important information for the subsequent modelling approach. To summarize, the present study represents the first holistic quantitative approach to determine bacterial overland transport. The state-of-the-art combination of quantitative, microbiological and molecular methods and parameters will provide the scientific basis for accurate prediction of BOT.

How to cite: Linke, R., Zhou, Y., Lindner, G., Hochenegger, N., Borovec, T., Reischer, G., Priselac, K., Hykollari, A., Stalder, G., Sommer, R., Derx, J., and Farnleitner, A.: From the pasture to the water: multiparametric laboratory experiments to determine microbial release from feces, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8224, https://doi.org/10.5194/egusphere-egu25-8224, 2025.

EGU25-10607 | ECS | Orals | HS1.1.4

Innovative modeling of the physicobiochemical determinants of fecal indicator bacteria 

Hao Wang, Anouk Blauw, Jos van Gils, Eline Boelee, and Gertjan Medema

The risk of infection by enteric pathogens in bathing waters is generally indicated by monitoring fecal indicator bacteria (FIB) concentrations. Mechanistic models are efficient tools for predicting FIB concentrations and corresponding contributions from various impact factors based on historical records and different climatic scenarios. However, most existing FIB physicobiochemical models are limited by the availability of FIB observations and knowledge of the physicobiochemical processes. Modeling studies that performed advanced sensitivity analyses or model comparisons to disentangle the contributions from different processes and impact factors, are rare.

To enhance the understanding of the relative importance of the various processes that affect FIB concentrations in different aquatic systems, we developed a comprehensive and generic FIB physicobiochemical model, including an improved die-off module and sediment interaction module. The new die-off module includes a cumulative endogenous photo-inactivation. By developing the relationship between dissolved organic carbon (DOC) concentrations and Ultraviolet diffuse attenuation coefficients, the module calculates the Ultraviolet-A (UVA) and Ultraviolet-B (UVB) extinction by waters. The penetrated UVA + UVB light under different wavelengths is used for endogenous photoinactivation rate calculation via the biological weighting function.  Distinct from using a constant partition rate in previous sediment interaction modules, the new sediment interaction module calculates the dynamic partition rate based on not only suspended sediment (SS) concentrations but also its composition via two different classes of SS: sand and clay.

Separate validation of the two sub-modules demonstrated the reliability of our modeling approach. Contrary to previous die-off modules, our new die-off module implied an improvement after adding UV endogenous photo-inactivation. According to sediment interaction module validation, the dynamic partitioning coefficient can reasonably allocate E. coli between water and sediment through sedimentation and resuspension, which is an essential precondition for incorporating sediment into the model as a reservoir for E. coli.

The sensitivity analysis result showed that 1) photo-inactivation is important in low DOC waters, but not in high DOC waters since the UV penetration is limited; 2) The impact of sediment interaction is insignificant under steady E. coli input conditions, but vital during and after a peak event. Interactions with sediments can extend the half-life of E. coli in water columns up to four times after a peak event.

This work demonstrated the significance of sediment interactions and DOC concentrations for predicting the duration of episodes of insufficient bathing water quality. The new generic module enables better simulation of bathing water quality across different types of aquatic environments and conditions. Future applications can choose processes selectively from the new FIB physicobiochemical model and couple it with hydrological or hydrodynamic models to address specific environmental conditions and research purposes.

How to cite: Wang, H., Blauw, A., van Gils, J., Boelee, E., and Medema, G.: Innovative modeling of the physicobiochemical determinants of fecal indicator bacteria, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10607, https://doi.org/10.5194/egusphere-egu25-10607, 2025.

EGU25-10696 | ECS | Orals | HS1.1.4

A Comparative Study of Arsenic Removal from Drinking Water Using Zero-Valent Iron (ZVI) and Magnetite/Reduced Graphene Oxide (MrGO) Coated Sand in Column Systems 

Acar Şenol, Sarp Çelebi, Omar A. I. M. Elkawefi, S. Sevinç Şengör, Gülay Ertaş, and Kahraman Ünlü

Arsenic contamination in drinking water is a pressing global issue, with over 250 million individuals lacking access to water that meets the World Health Organization's recommended limit of 10 µg/L. Arsenic, a confirmed carcinogen, poses significant health risks, necessitating efficient and cost-effective removal strategies. Adsorption remains one of the most prevalent methods for arsenic removal, employing materials such as metal oxides, graphene-based metal oxides, nanocomposites, and carbonaceous materials and organic-metallic frameworks. One of the most researched materials for the removal of arsenic from drinking water is Zero-Valent Iron (ZVI).  However, ZVI, while widely utilized, exhibits limitations including reduced efficacy for As(III), extended reaction times, sensitivity to competing ions, narrow operational pH and DO range, and iron leaching into the water. This study explores the potential of magnetite/reduced graphene oxide (MrGO)-coated sand as an advanced alternative. MrGO's structural synergy, combining highly adsorptive magnetite nanoparticles with the enhanced stability and properties of reduced graphene oxide, addresses many of ZVI’s shortcomings. However, its application in column studies as a fixed nanoparticle remains underexplored, limited to theoretical and batch studies and pelletized or layered column studies. A novel approach to arsenic removal by integrating MrGO-coated sand and ZVI in column systems is presented in this work. The study evaluates their performance independently and in combination, focusing on removal efficiency, operational range, and cost-effectiveness. This includes the development of MrGO-coated sand for enhanced applicability in column systems and the optimization of MrGO-to-ZVI ratios to achieve maximum removal efficiency under conditions representative of real-world groundwaters. Preliminary findings suggest that MrGO-coated sand demonstrates the ability of the material to adequately remove arsenic while maintaining a broader operational conditions compared to ZVI. By investigating optimal ratios and conditions, this study aims to balance performance with economic feasibility, providing a scalable solution for arsenic-contaminated water treatment, contributing to the advancement of arsenic removal technologies and highlighting the potential of reduced-graphene-oxide-based materials in addressing critical water quality challenges.

How to cite: Şenol, A., Çelebi, S., Elkawefi, O. A. I. M., Şengör, S. S., Ertaş, G., and Ünlü, K.: A Comparative Study of Arsenic Removal from Drinking Water Using Zero-Valent Iron (ZVI) and Magnetite/Reduced Graphene Oxide (MrGO) Coated Sand in Column Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10696, https://doi.org/10.5194/egusphere-egu25-10696, 2025.

EGU25-11562 | Orals | HS1.1.4 | Highlight

Temporal modeling of surface water bacteriological quality in West Africa using remote sensing and machine learning methods 

Marc-Antoine Mant, Elodie Robert, Manuela Grippa, Laurent Kergoat, Moussa Boubacar moussa, Beatriz Funatsu, Javier Perez Saez, Rochelle Newall Emma, and Marc Robin

In 2021, diarrheal diseases were responsible for around 1.17 million deaths worldwide. Sub-Saharan Africa is one of the most impacted regions, where 440,000 deaths were recorded in 2024. This high mortality rate can be explained by 1) significant bacteriological pollution of surface waters by pathogenic micro-organisms responsible for diarrheal diseases, 2) widespread use of untreated water by the population and3) lack of sanitation and community health infrastructures. In addition, ongoing climate change is likely to have a negative impact on water quality, and potentially increase the presence and transmission of pathogens.

Tele-epidemiology, the combination of satellite observations and epidemiology, is a powerful tool for studying climate-environment-health relationships and for understanding and predicting the spatio-temporal distribution of pathogens and diseases through the use of satellite and in-situ data. We aim at using this method to indirectly monitor water quality and reveal environmental factors conducive to the emergence of critical health situations by modeling the dynamics of E. coli in West Africa. E. coli is considered the best indicator of faecal contamination (IFC) in temperate zones, and is recommended as a proxy for assessment of water contamination. In Burkina Faso, Robert et al (2021) demonstrated a significant correlation between E. coli, intestinal enterococci and cases of diarrhea. E. coli therefore appears to be a good IFC in West Africa, and would be relevant for predicting diarrheal diseases.

The first objective is to study the links between E. coli concentration in water and environmental parameters 1) measured in-situ in West African surface waters (Bagre reservoir in Burkina Faso and Kongou - Bangou Kirey in Niger) from 2018 to 2024 (concentration of suspended particulate matter, particulate organic carbon, etc.), 2) measurable by satellite (surface water reflectances mesured by Sentinel-2) or 3) estimable by satellite algorithm (precipitation, hydrometeorological parameters, NDVI, etc.). We then use key environmental parameters to model the concentration of E. coli in these sites over several years, firstly using all parameters, and then only using satellite data to study their robustness. Various machine learning models (Random Forest, SVM, KNN, etc.) were tested and compared with each other (calculation of R², RMSE, MSE and MAPE). 

For the Bagre site, the best model of E. coli concentration had showed a R² of 0.76 (RMSE 0.49 log10 MPN/100mL) using in-situ and satellite data, and R² of 0.69 with only satellite data (RMSE 0.56 log10 MPN/100mL). For Kongou, the best model had showed a R² of 0.7 using in-situ and satellite data, and R² of 0.65 with only satellite data.

This work will allow to create health hazard indices that can be used by public health players, firstly in West Africa without the need to collect data in the field, and then more generally for other sites facing similar public health problems.

How to cite: Mant, M.-A., Robert, E., Grippa, M., Kergoat, L., Boubacar moussa, M., Funatsu, B., Perez Saez, J., Emma, R. N., and Robin, M.: Temporal modeling of surface water bacteriological quality in West Africa using remote sensing and machine learning methods, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11562, https://doi.org/10.5194/egusphere-egu25-11562, 2025.

EGU25-12690 | ECS | Posters on site | HS1.1.4

Multiparametric Modeling of Bacterial Release and Overland Transport from Feces: Insights from Rainfall Experiments and Molecular Diagnostic Tools  

Yanhe Zhou, Rita Linke, Regina Sommer, Gerhard Lindner, Peter Strauss, David Ramler, Alba Hykollari, Gabrielle Stalder, Raphael Anton Schatz, Katarina Priselac, Mats Leifels, Margaret Stevenson, Katalin Demeter, Alfred Paul Blaschke, Jack Schijven, Andreas Farnleitner, and Julia Derx

Water contamination caused by enteric microbial pathogens from humans and animals poses serious risks to public health. Rainfall events can induce the release of microorganisms from feces, and the health risks posed by these pathogens to water bodies are highly dependent on their transport and survival characteristics. Novel molecular tools and diagnostic capabilities have rapidly advanced in recent years, offering significant potential to revolutionize the study of microbial contamination and transport in water bodies and to enhance the modeling of overland transport of microorganisms through the application of these advanced diagnostic methods. This study employs rainfall-release experiments and pathogen enumeration in runoff and infiltrated water to investigate bacterial release and overland transport mechanisms from fresh cow feces, aiming to address gaps in advanced molecular techniques and to assess the impacts of fecal shape and aging on the precise quantification of bacterial overland transport (BOT).

Artificial rainfall experiments are conducted on fresh cow pat samples which are placed onto bare surfaces to study bacterial release and onto small scale undisturbed soil plots to study bacterial overland transport. The experimental setup includes three rainfall intensities (40 mm/h, 60 mm/h and 80 mm/h) and two slopes (5% and 25%). In addition, the effects of different fecal shapes are investigated (large and small surface area-to-volume ratios). The quantitative analyses are done for different microbial parameters (FIB, bacterial MST markers) using both culture-based and qPCR-based methods and the effects of experimental setups, microbial parameters, and enumeration methods will be compared and evaluated. The release will be modelled using the Bradford-Schijven model formulations, and Kineros2/STWIR will be used for modelling the BOT.

This study will improve the understanding of the release and transport of manure-borne pathogens from fresh cow pats and provide a more precise quantitative approach to measuring BOT using advanced diagnostic methods.

How to cite: Zhou, Y., Linke, R., Sommer, R., Lindner, G., Strauss, P., Ramler, D., Hykollari, A., Stalder, G., Anton Schatz, R., Priselac, K., Leifels, M., Stevenson, M., Demeter, K., Paul Blaschke, A., Schijven, J., Farnleitner, A., and Derx, J.: Multiparametric Modeling of Bacterial Release and Overland Transport from Feces: Insights from Rainfall Experiments and Molecular Diagnostic Tools , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12690, https://doi.org/10.5194/egusphere-egu25-12690, 2025.

EGU25-12827 | Orals | HS1.1.4

 Estimate public exposure to PAHs and environmental risks through wastewater-based epidemiology 

Katarzyna Styszko, Justyna Pamuła, Elżbieta Sochacka-Tatara, Agnieszka Pac, and Barbara Kasprzyk-Hordern

 Waterwater-based epidemiology (WBE) may be able to monitor public health emergencies by analyzing human urinary biomarkers in wastewater. This work proposes a novel approach utilizing WBE for the spatial and temporal evaluation of PAHs exposure using hydroxyl derivatives of PAHs. These are 1-hydroxynaphthalene, 2-hydroxynaphthalene, 2-hydroxyfluorene, 9-hydroxyfluorene, 9-hydroxyphenanthrene, 1-hydroxypyrene and 3-hydroxybenzo(a)pyrene. Most target markers were found at quantifiable concentrations in raw and treated wastewater. The total loads identified in raw sewage ranged from 88.33 g/day  to 154.77 g/day during the summer period and from 137.66 g/day to 283.78 2 g/day during the winter period. The obtained results for the removal efficiencies of OH-PAHs indicate a seasonal dependency in their degradation. Removal efficiencies were higher in January compared to August.

The results of the back calculations allowed to estimate that during the summer, on average, a resident of Krakow could absorb approximately 2.1 µg of the assessed OH-PAHs per day, while in winter, this value increased to 4.1 µg. This is close to the reported in the literature value that the total daily exposure to OH-PAHs is estimated at 3 µg/day.

Moreover, the risk quotation (RQ) values on the base of acute and chronic data base for compounds present in effluents were calculated. The RQ values in January were relatively low, but in August the RQ values were higher, indicating a high concentration of effluent and nitrogen in summer as these compounds were removed in winter and summer.

To the authors’ knowledge, this is the first time wastewater profiling of OH-PAHs in wastewater for the evaluation of exposure to PAHs have been used, also their removal as well emission with effluent were determined. 

How to cite: Styszko, K., Pamuła, J., Sochacka-Tatara, E., Pac, A., and Kasprzyk-Hordern, B.:  Estimate public exposure to PAHs and environmental risks through wastewater-based epidemiology, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12827, https://doi.org/10.5194/egusphere-egu25-12827, 2025.

EGU25-13044 | ECS | Posters on site | HS1.1.4

Stability of selected nitrification and urease inhibitors in surface water 

Lisa Michael, Eleonora Flores, Silke Pabst, and Sondra Klitzke

Nitrification (NI) and urease inhibitors (UI) are added as organic trace substances to agricultural land during the application of nitrogen and urea fertilizers. They inhibit the nitrification processes and urease activity in soil and thus ensure a reduced emission of gaseous ammonia and nitrous oxide. The application of UI has been mandatory since 2020 following the amendment to the German Fertilizer Ordinance, which means that increased use is to be expected. The substances can enter surface waters through translocation and leaching processes in soils. So far, the stability of NI and UI in the aqueous phase has only been investigated in ultrapure water and tap water. Therefore, the aim of this study was to investigate the stability of five NI, i. e. 1H-1,2,4-triazoles (triazole), dicyandiamides (DCD), 3,4-dimethylpyrazoles (3,4-DMP), 3-methylpyrazoles (3-MP), N-((3(5)-Methyl-1H-pyrazol-1-yl)methyl)acetamid (MPA) and one UI, i. e. N-(2-nitrophenyl)phosphoric acid triamide (2-NPT), in two natural surface waters at 20 °C and at different pH values (i. e. pH 5, 7 and 9) using batch experiments. We distinguished between the processes of hydrolysis, sorption and microbial degradation. Hence, three differently treated triplicate batch samples were set up after the removal of suspended matter (> 0.63 mm). To investigate hydrolysis, the test water was filtered through a 0.22 μm polyamide membrane. For the investigation of sorption on suspended solids, a sodium azide solution was added to the water to inactivate microorganisms (final concentration in batch samples 100 mg/L). To investigate microbial degradation, the test water was used in its natural composition. pH values were adjusted using dilute HNO3 and NaOH, respectively. The six inhibitors were added as a mixture to each batch sample with a target concentration of 5 μg/L each. Batch samples were taken, subsequently filtered (0.45 µm, regenerated cellulose) and measured by HPLC-MS/MS over a period of 8 days for the sorption tests and 83 days for the hydrolysis and microbiological degradation experiments.

None of the investigated inhibitors showed any sorption on suspended solids. With regard to hydrolysis and microbial degradation, the results differed depending on inhibitor and pH. For MPA no decomposition by hydrolysis could be detected at all three pH values. However, MPA was microbially degraded at pH 7 and pH 9 and was no longer detectable after about 55 days. 2-NPT was hydrolytically degraded at pH 5 and 9 over the entire test period, but no hydrolysis was observed at pH 7. At pH 7, no microbial degradation could be detected for 70 days. Thus, 2-NPT is persistent at pH 7. At pH 9, our results did not show any microbial degradation for 2-NPT. The stability of inhibitors in surface waters is driven by hydrolysis and microbial degradation and may vary greatly with pH.

How to cite: Michael, L., Flores, E., Pabst, S., and Klitzke, S.: Stability of selected nitrification and urease inhibitors in surface water, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13044, https://doi.org/10.5194/egusphere-egu25-13044, 2025.

EGU25-13064 | ECS | Posters on site | HS1.1.4

Fate of urease and nitrification inhibitors in surface water and saturated sediment 

Antonia Zieger, Eleonora Flores, Silke Pabst, and Sondra Klitzke

Nitrification and urease inhibitors (NI,UI) added to fertilisers can increase the availability of nitrogen to plants. By inhibiting certain processes, they could contribute to a reduction in the emission of N2O and NH3 compounds and a reduction in nitrate leaching. Some of these substances have already been detected in surface water and groundwater and are considered to be harmful to human health. The inhibitors are therefore an area of conflict between climate change mitigation and increased fertiliser efficiency on the one hand, and soil and groundwater protection on the other. However, knowledge of their abiotic and biotic degradation in water and saturated sediment systems is currently very limited.

The aim of this study is to determine the fate of the 6 most commonly used inhibitors 1H-1,2,4-Triazol (Triazole), Dicyandiamide (DCD), 3,4-Dimethylpyrazol (3,4-DMP), N-[(3 or 5-methyl-1H-pyrazol-1-)methyl]acetamid (MPA), 3-Methylpyrazol (3-MP) and N-(2-Nitrophenyl) phosphoric triamide (2-NPT) in surface water and saturated sandy sediments.

Triplicate batch samples containing either saturated water-sediment mixtures (solid-solution-ratio 1:3) or surface water only were spiked with six inhibitors (target concentration 1.5 µg/L each). Both sets were maintained under biotic or abiotic (autoclaved water and sediment) conditions at room temperature. The supernatant was sampled periodically for 90 days and analysed for inhibitors, pH, dissolved organic carbon and electrical conductivity.

None of the inhibitors were sorbed to the sediment except Triazole, which showed only minimal sorption of less than 10%. The urease inhibitor 2-NPT was partly decomposed by hydrolysis alone under the studied pH between 7-8.6. Degradation in general was most pronounced in the biotic water-sediment mixture where DCD and MPA were completely degraded and 3,4-DMP, 2-NPT and 3-MP were partially degraded. The Inhibitor MPA was very susceptible to biodegradation even in surface water, however, its forming metabolite 3-MP is not. Triazol was not degraded under any conditions in this study.

With the exception of Triazole, saturated sediments (for instance in a bank filtration scenario) could probably reduce most of the inhibitors’ concentrations if the microbial community is intact. However, four out of six inhibitors were not completely degraded even under biotic conditions within 90 days, making them susceptible to breakthroughs into groundwater. Therefore, their fate in the environment should be studied further.

How to cite: Zieger, A., Flores, E., Pabst, S., and Klitzke, S.: Fate of urease and nitrification inhibitors in surface water and saturated sediment, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13064, https://doi.org/10.5194/egusphere-egu25-13064, 2025.

Cigarette smoking and its negative health effects are well documented; however, the environmental impacts of cigarettes are poorly understood. Moreover, considering cigarette butts (CBs) as one of the most littered items globally, exploring the relative environmental effects of different end-of-life (EoL) pathways is essential to design effective mitigation strategies. So, the objective of this study is to identify the environmental hotspots across the cigarette lifecycle—both upstream and downstream of consumption—and to compare the environmental impacts of three potential EoL pathways of the CBs using a comprehensive cradle-to-grave life cycle assessment (LCA). The results depicted that cigarette manufacturing accounted for the highest environmental impact (98.36%) among the upstream processes of the cigarette life cycle. Especially human carcinogenic toxicity emerged as the highest potent impact category (0.168 kg 1,4-DCB), followed by freshwater eutrophication (0.0014 kg P eq.) and freshwater ecotoxicity (0.0525 kg 1,4-DCB) for a single cigarette production. Additionally, the cigarette consumption phase also depicted the highest environmental impacts contributing to human carcinogenic toxicity (96.3%), primarily due to the release of hazardous air pollutants during smoking. Further, the relative environmental impacts of three EoL scenarios were analysed for a CB—incineration, littering and landfilling disposal. Among the EoL scenarios analysed, littering of CBs caused the highest environmental impacts, mainly due to the leaching of toxic contaminants into water bodies. Despite evidence that CBs contain over 150 highly toxic chemicals with carcinogenic and mutagenic properties, the lack of detailed, standardized databases for these substances limits the precision of environmental impact analyses. Future research should address this gap by developing comprehensive databases and standardized methodologies to incorporate the specific contaminants in CBs. Such advancements are essential for a more accurate and holistic evaluation of the environmental pollution associated with CB disposal and to guide effective mitigation strategies.

How to cite: Lourembam, N. and Vanapalli, K. R.: Life cycle assessment of Cigarette from cradle to grave: Identifying environmental hotspots and end-of-life scenario analysis, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15223, https://doi.org/10.5194/egusphere-egu25-15223, 2025.

EGU25-16997 | Posters on site | HS1.1.4

Pesticide contamination across drinking water sources in the Netherlands 

Arnaut van Loon, Inge van Driezum, Tessa Pronk, and Sharon Clevers

Pesticides have been found in surface water and groundwater sources for decades. They are not only widely considered as a major threat for these waters, but also for drinking water. Not only pesticides that are still authorized by the European Commission can be found in the sources for drinking water, also banned compounds, such as atrazine (banned in 2007), still cause exceedances of environmental threshold values (as measured in 2020).

A comprehensive study was conducted in Dutch drinking water sources analyzing pesticides and their metabolites in both surface water and groundwater. Observations in surface water sources were divided in intake water and pre-treated water. For groundwater sources, observations were divided in observation wells, individual abstraction wells and all abstraction wells per particular drinking water abstraction station. Dutch drinking water standards were used as a measure of the implications for drinking water production processes.

This study shows that 156 different pesticides or metabolites were found at the nine surface water intake points considered. The standard for this substance group was exceeded on several occasions at all intake points. Pesticide residues have also been found in 40% of groundwater abstractions for drinking water production, particularly in phreatic ones (77%). This also involves a diversity of different substances. Pesticide residues exceeded the standard in 20% of groundwater abstractions. The pressure on surface water quality due to pesticides as indicated by the Removal Requirement Index seems to decrease slightly in recent years, whereas the pressure on groundwater intended for drinking water production seems to increase. Due to the diversity of pesticides found in ground- and surface water, trends are not obvious. Which and how many pesticides were observed differs between observation wells, abstraction wells and the combined abstraction wells, as well as aquifer properties.

How to cite: van Loon, A., van Driezum, I., Pronk, T., and Clevers, S.: Pesticide contamination across drinking water sources in the Netherlands, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16997, https://doi.org/10.5194/egusphere-egu25-16997, 2025.

EGU25-19192 | Orals | HS1.1.4

Development and Validation of a GIS-Based Tool for Disinfection Byproduct Formation Prediction in Water Distribution Systems 

Demetrios G. Eliades, Stelios G. Vrachimis, Pavlos Pavlou, and Marios Kyriakou

Disinfection of water in distribution systems is essential for ensuring the microbiological safety of drinking water. However, disinfection byproducts (DBPs) are chemical compounds formed when disinfectants, such as chlorine, react with natural organic matter (NOM) and other constituents in water. The formation of DBPs in drinking water distribution systems can pose health risks, including cancer and reproductive issues, necessitating robust strategies to predict and mitigate their presence.

As part of the EU-funded IntoDBP project, a comprehensive real-world case study was conducted in Limassol, Cyprus, to investigate DBP formation within a water distribution system. The study included monitoring the hydraulic and water quality states of the system, from the Drinking Water Treatment Plant (DWTP) to end-users. This complete system perspective allowed for the evaluation of key factors affecting DBP formation, such as water source characteristics, residence time, and chlorination practices.

This work presents the process of creating a DBP modeling tool, detailing the methods used to address challenges related to the integration of heterogeneous data sources. Data from the DWTP, re-chlorination points, and distribution nodes were harmonized to ensure accurate representation of both hydraulic conditions and chemical reactions. Models capable of predicting DBP formation were developed as part of the study, with a specific focus on trihalomethanes (THMs) and haloacetic acids (HAAs). These models were validated using real-time data from sensors and manual sampling.

Alongside these models, a GIS-based software tool was developed to explore strategies for minimizing DBP levels within distribution networks. This tool visualizes data from multiple sources, including SCADA systems, water quality sensors, and GIS data, enabling dynamic simulations and scenario testing. Advanced simulation techniques using EPANET-MSX facilitated the simulation of multi-species reactions and the incorporation of uncertainties, such as variations in source water composition and operational conditions. The tool provides researchers and practitioners with the capability to evaluate and optimize chlorination practices, water mixing strategies, and operational configurations to mitigate DBP risks effectively.

Results from the case study highlighted the critical role of water residence time and source water composition in DBP formation. Nodes farther from chlorination points and those receiving water with higher NOM levels exhibited elevated DBP concentrations, emphasizing the importance of optimizing hydraulic and chemical parameters throughout the distribution system. The developed software tool demonstrated the potential of integrating GIS and hydraulic data with chemical analyses. It also showed promise in evaluating various mitigation strategies, including dynamic chlorination schedules and adjustments in flow management, within a realistic setup. This tool offers a valuable resource for researchers and water utility operators, providing a benchmark platform for developing and validating innovative DBP management strategies.

How to cite: Eliades, D. G., Vrachimis, S. G., Pavlou, P., and Kyriakou, M.: Development and Validation of a GIS-Based Tool for Disinfection Byproduct Formation Prediction in Water Distribution Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19192, https://doi.org/10.5194/egusphere-egu25-19192, 2025.

EGU25-19916 | Orals | HS1.1.4

AMR pollution dynamics determined by the untreated wastewater domination of both the hydrology and point source loads to the Musi River, Hyderabad 

Joshua Larsen, Vikas Sonkar, Arun Kashyap, Rebeca Pallarés-Vega, Ankit Modi, Cansu Uluseker, Pranab Mohapatra, David Graham, and Jan-Ulrich Kreft

Antimicrobial resistance (AMR) is a silent pandemic, which is transmitted and spread through the environment. Throughout the global south, large urban areas interact with, and often exert considerable control on, both the hydrological and pollution dynamics on the rivers they are built around. Despite this, little is known about the prevalence, sources, and transport of AMR through these common, yet complex environments. Here, we quantified taxonomic and resistance genes (ARGs), sensitive and resistant bacteria (ARBs), and environmental conditions in both river water and sediment along the Musi River in Hyderabad, a city renowned for antimicrobial manufacturing and urban dominance of the river environment. We also developed estimates of urban wastewater inputs and a hydraulic model to understand the rapid changes in river flow and pollution concentrations occurring along the river length through the city. This reveals increasing, though variable, concentrations in ARGs along the river through the dry season, and stronger discrete point source and flow dilution dynamics in the wet season. The riverbed sediment stores far higher concentrations than the water column, especially in the dry season, and has more dynamic interaction with the river during the wet season. This study reveals the importance of both flow and removal dynamics in controlling AMR prevalence in the environment, in a context that is both common and expanding throughout the global south.

How to cite: Larsen, J., Sonkar, V., Kashyap, A., Pallarés-Vega, R., Modi, A., Uluseker, C., Mohapatra, P., Graham, D., and Kreft, J.-U.: AMR pollution dynamics determined by the untreated wastewater domination of both the hydrology and point source loads to the Musi River, Hyderabad, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19916, https://doi.org/10.5194/egusphere-egu25-19916, 2025.

EGU25-21206 | Orals | HS1.1.4

Co-occurrence of antibiotics, antimicrobial resistance genes and wastewater indicators in surface waters near Bangkok, Thailand: Characterization, Distribution & Controls 

Laura Richards, George J. L. Wilson, Ajmal Roshan, Farah T. Ahmed, Mariel Perez-Zabaleta, Santiago Nicolás Otaiza-González, Sara Rodríguez-Mozaz, Zeynep Cetecioglu, and David A. Polya

Aquatic pollution from emerging contaminants, including antibiotics and antimicrobial resistance (AMR) genes, is an important environmental concern particularly pertinent in megacities such as Bangkok, Thailand, impacted by rapid urbanization and massive water demand.  Using a suite of environmental and hydrogeochemical tracers including inorganics and organics, nutrients, metal(loids), select antibiotics and AMR genes [1, 2], we characterize the distribution and spatial patterns of a range of contaminants in a ~ 150 km transect of the Chao Phraya River Basin in Thailand capturing areas both upstream and downstream of Bangkok.  A range of antibiotics and AMR genes were identified in parts of the transect and downstream trends are investigated.  Co-occurrence between selected antibiotics and AMR genes was not statistically significant, although other significant hydrogeochemical relationships (e.g. between pH and selected AMR genes) were observed, suggesting complex controls and selection pressures.  Comparisons are made with the types and concentrations of similar compounds detected in other major river and groundwater systems near other rapidly developing cities in South Asia (e.g. Patna, India) [3-5].  This work highlights the added interpretive value of a comprehensive range of analytes and provides insight on the potential co-occurrence of antibiotics, antimicrobial resistance genes and wastewater indicators that may be observed in surface waters in such settings.

Acknowledgements: We acknowledge support from a UKRI ODA allocation (via UoM to DP et al), a UoM-KTH strategic partnership seedcorn award (to LAR & ZC), a UKRI Future Leaders Fellowship (MR/Y016327/1 to LAR et al), a DKOF (to LAR), Cookson Studentship (to AR), and the Resistomap team.

References: [1] Larsson & Flach, Nature Reviews Microbiology, 2022, https://doi.org/10.1038/s41579-021-00649-x; [2] Hutinel et al., Science of the Total Environment, 2022, https://doi.org/10.1016/j.scitotenv.2021.151433; [3] Wilson et al., Environmental Pollution, 2024, https://doi.org/10.1016/j.envpol.2024.124205; [4] Richards et al., Environmental Pollution, 2023, https://doi.org/10.1016/j.envpol.2023.121626; [5] Richards et al., Environmental Pollution, 2021, https://doi.org/10.1016/j.envpol.2020.115765.

How to cite: Richards, L., Wilson, G. J. L., Roshan, A., Ahmed, F. T., Perez-Zabaleta, M., Otaiza-González, S. N., Rodríguez-Mozaz, S., Cetecioglu, Z., and Polya, D. A.: Co-occurrence of antibiotics, antimicrobial resistance genes and wastewater indicators in surface waters near Bangkok, Thailand: Characterization, Distribution & Controls, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21206, https://doi.org/10.5194/egusphere-egu25-21206, 2025.

EGU25-21831 | Orals | HS1.1.4

Pathogen removal in sandy aquifers: lessons from multiple field and column studies for safe water supply

Gertjan Medema, Bas van der Zaan, Martin van der Schans, and Gijsbert Cirkel

EGU25-1388 | Posters on site | ST1.7

Platform of adaptive algorithms for global simulations of planetary space weather 

Ilja Honkonen, Riku Jarvinen, and David Phillips

We present a new free and open source (FOSS) simulation platform under development at the Finnish Meteorological Institute. Building on top of our existing space weather models for Earth, Mercury and other planets, the aim is to enable efficient global simulations of plasma interactions in the solar system and beyond, including unmagnetized and magnetized planetary bodies with and without atmospheres and ionospheres. Our development focuses on a flexible combination of magnetohydrodynamic (MHD), hybrid particle-in-cell (PIC) and full-kinetic methods. Fast time to solution is achieved via runtime adaptive mesh refinement (AMR), temporal substepping and massively parallel implementation using the message passing interface (MPI) and open multi-processing (OpenMP). We describe our approaches to combining different physical solutions within the same simulated volume and combining AMR with substepping. We verify the implementation against a plethora of test cases in one, two and three dimensions, and also discuss initial results from simulations of Mercury and BepiColombo flybys using particle and MHD approaches and highlight the largest differences.

How to cite: Honkonen, I., Jarvinen, R., and Phillips, D.: Platform of adaptive algorithms for global simulations of planetary space weather, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1388, https://doi.org/10.5194/egusphere-egu25-1388, 2025.

EGU25-1415 | ECS | Posters on site | ST1.7

Plasma waves in a global ion-kinetic hybrid simulation for Mercury's space weather 

David Phillips, Riku Jarvinen, Ilja Honkonen, and Esa Kallio

We present analyses of plasma wave modes in our global hybrid particle-in-cell simulation code, RHybrid, for flowing planetary plasma interactions. The model treats ions as macroscopic particle clouds moving under the Lorentz force while electrons are a charge-neutralising, massless fluid. Magnetic field is advanced by Faraday's law and coupled self-consistently with ion dynamics (ion charge density and ion electric current density) via non-radiative Maxwell's equations. We describe analyses of several test cases, like random initial conditions and backstreaming suprathermal populations, compared against known solutions, observations and previous results from local and global modeling, including Mercury-type solar wind and interplanetary magnetic field conditions. The results show dispersion relations, parameter correlations, polarisations and more. We discuss the accuracy of modelling of theoretical results, including properties of whistler, Alfvén and magnetosonic waves, and ion-ion streaming instabilities in RHybrid. With this work, we prepare for further development of the Finnish Meteorological Institute's free and open source space weather particle simulation platforms, and for the interpretation of upcoming observations from the BepiColombo mission.

How to cite: Phillips, D., Jarvinen, R., Honkonen, I., and Kallio, E.: Plasma waves in a global ion-kinetic hybrid simulation for Mercury's space weather, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1415, https://doi.org/10.5194/egusphere-egu25-1415, 2025.

EGU25-2097 | ECS | Posters on site | ST1.7

The role of nonthermal electron distribution in triggering electrostatic ion-acoustic instability near the Sun 

Mahmoud Saad Afify, Jürgen Dreher, Stuart O'Neill, and Maria Elena Innocenti

Discoveries by Parker Solar Probe (PSP) highlight the significance of nonthermal distributions in triggering ion-scale instabilities (Verniero et al. 2020, 2022; An et al. 2024; Liu et al. 2024). In this study, we show how the electron nonthermal (kappa) distribution could change the onset threshold of the ion-acoustic instability (IAI) recently observed by PSP (Mozer et al. 2021, 2023; Kellogg et al. 2024) between 15 and 25 solar radii and modeled by Afify et al. (2024). We perform analytical studies and kinetic simulations using the Vlasov-Poisson code with a parameter regime relevant to PSP observations. A setup of kappa-distributed electrons and two counterstreaming Maxwellian ion distributions (a core and a beam) is shown to be unstable w.r.t. the IAI, however, the electron-to-core and beam-to-core temperature ratios are slightly different from those recorded by PSP. The simulated growth rates have been validated by the kinetic theory. In the saturation regime, we do observe the formation of ion holes in the beam phase-space density. With large kappa values, the ion-acoustic waves interacted substantially with the beam, for instance, κ = 20, and shifted away from the beam with lower kappa values, for instance,  κ = 5 and 7. Our findings confirm that protons exhibit reduced resonance in the presence of kappa electrons, and the electron heating observed by PSP during the presence of IAI is not replicated in our simulation (Mozer et al. 2022).

References

Afify, M. A., Dreher, J., Schoeffler, K., Micera, A., & Innocenti, M. E. 2024, APJ, 971, 93
An, X., Artemyev, A., Angelopoulos, V., et al. 2024, PRL, 133, 225201.
Kellogg, P. J., Mozer, F. S., Moncuquet, M., et al. 2024, ApJ 964, 68.
Liu, W., Jia, H., & Liu, S. 2024, AJL 963, L36.
Mozer, F., Bale, S., Kellogg, P., et al. 2023, Phys. Plasmas, 062111, 30
Mozer, F. S., Bale, S. D., Cattell, C. A., et al. 2022, AJL 927, L15.
Mozer, F. S., Vasko, I. Y., & Verniero, J. L. 2021, ApJL, 919, L2.
Verniero, J. L., Chandran, B. D. G., Larson, D. E., et al. 2022, ApJ, 924, 112
Verniero, J. L., Larson, D., Bowen, T. A., et al. 2020, ApJS, 248, 5

How to cite: Afify, M. S., Dreher, J., O'Neill, S., and Innocenti, M. E.: The role of nonthermal electron distribution in triggering electrostatic ion-acoustic instability near the Sun, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2097, https://doi.org/10.5194/egusphere-egu25-2097, 2025.

A flattop distribution is one of the most characteristic non-Maxwellian velocity distributions in space plasmas. It is often observed in collisionless shocks and reconnection sites in near-Earth space. In this contribution, we discuss a numerical approach to study a flattop plasma in particle-in-cell (PIC) simulations. Specifically, we propose two numerical methods for randomly generating flattop-distributed velocities: a piecewise rejection method and a transform method from a gamma-distributed random number. Their usability is briefly compared.
Gamma-distributed random numbers are useful for generating flattop and other distributions. However, random number generators (RNGs) for gamma distribution may not be always efficient. Here, we propose a novel RNG algorithm for gamma distribution with shape parameter less than unity, based on the generalized exponential distribution and the squeeze method [1]. Numerical tests show that the proposed method is one of the best two in this category.

[1] S. Zenitani, Economics Bulletin, 44, 1113-1122 (2024), arXiv:2411.01415

How to cite: Zenitani, S.: Random number generation in kinetic plasma simulation: flattop and gamma distributions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2192, https://doi.org/10.5194/egusphere-egu25-2192, 2025.

The magnetohydrodynamic model of the solar high-temperature atmosphere is an important plasma model, which can reproduce many important features in simulating solar coronal plasma and magnetic field processes. However, the assumption of the MHD model may fail during highly dynamic and transient events, such as magnetic reconnection, and plasma heating, and in partially ionised structures such as the chromosphere, sunspots, and coronal rain. Therefore, a two-fluid MHD model with ions and neutral components can simulate many new phenomena. This study considers the two- fluid effects of solar plasma, and investigates the modification to traditional MHD models by including neutral components. We simulated MHD waves, and loop top turbulences in partially ionised plasma in sunspots or chromospheric flows. We focus on the separation of ions and neutral components in energy transfer processes and the potential contribution of neutral components to the nascent solar wind. Our simulations show that two-fluid effects would contribute significantly to solar plasma heating by collisional friction, and lead to the leakage of neutral components across the magnetic field lines and escape to the corona, it completely revolutionised our understanding of the corona, in which the role of the neutral component was neglected.

How to cite: Yuan, D. and Kuzma, B.: Two-fluid magnetohydrodynamic effects in the high-temperature atmosphere of the sun and their new perspectives, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2724, https://doi.org/10.5194/egusphere-egu25-2724, 2025.

EGU25-3036 | ECS | Posters on site | ST1.7

Magnetohydrodynamic wave as a tool for solar plasma diagnostics and heating 

Libo Fu, Ding Yuan, Błażej Kuźma, and Yuandeng Shen

Magnetohydrodynamic (MHD) waves interact with the solar magnetic structures and have the potential to heat solar plasma and be used as a tool for plasma diagnostics. Despite extensive research, the precise mechanisms by which waves contribute to energy transport and dissipation remain incompletely understood. Additionally, utilizing wave characteristics for accurate diagnostics of the coronal plasma structure presents a significant challenge. Here, we utilize the Goode Solar Telescope to demonstrate transverse oscillations of the dark fibrils within the umbra of a sunspot and investigate their role in plasma heating. Additionally, we use EUV observations to show a quasi-periodic fast-mode MHD wave passing through a coronal hole could serve as a tool for plasma diagnostics. Our study finds that transverse oscillations are prevalent in the umbra of sunspots and carry a wave energy flux that significantly exceeds the loss rate of the solar active regions. Furthermore, the discovery of the MHD wave lensing effect provides a new mechanism for coronal hole diagnostics, with potential application to polar regions. These findings confirm the crucial role of MHD waves in coronal heating and demonstrate their potential as diagnostic tools for coronal plasma parameters. The studies provide new perspectives for understanding the multi-scale energy conversion and wave-magnetic field interactions in the solar atmosphere.

How to cite: Fu, L., Yuan, D., Kuźma, B., and Shen, Y.: Magnetohydrodynamic wave as a tool for solar plasma diagnostics and heating, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3036, https://doi.org/10.5194/egusphere-egu25-3036, 2025.

EGU25-3046 | Orals | ST1.7

The role of current helicity in driving solar dynamo 

Mei Zhang and Yuhong Fan

A series of numerical simulations of convective dynamo, with varying grid resolution, with or without explicit magnetic diffusivity and viscosity, are presented and analyzed. It is found that in the simulations, with the increase of Reynolds number, the magnitude of current helicity increases dramatically, whereas the variation of kinetic helicity is very moderate. The competition between the kinetic helicity term and the current helicity term of the alpha coefficient results in an interesting behavior of the large-scale magnetic fields that resembles the ``dynamo-disappear-and-recover" phenomena reported in Hotta et al. 2016 Science paper. Our simulation and analysis suggest that, the role of current helicity first functions to suppress the dynamo, as the convectional $\alpha$-quenching concept states, but then functions to drive the dynamo, instead of quenching it, after a critical Reynolds number is exceeded.

How to cite: Zhang, M. and Fan, Y.: The role of current helicity in driving solar dynamo, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3046, https://doi.org/10.5194/egusphere-egu25-3046, 2025.

EGU25-3962 | ECS | Posters on site | ST1.7

A Novel Poloidal-Toroidal Approach for Spherical Force-Free Field Reconstruction of Coronal Magnetic Fields 

Sibaek Yi, Gwang-Son Choe, Sunjung Kim, and Minseon Lee

Understanding solar eruptive phenomena requires accurate information about the coronal magnetic field. However, due to current technological limitations, direct measurement of the coronal magnetic field in three dimensions remains nearly impossible. Consequently, it is often approximated as a force-free field (FFF) using vector magnetogram data, which provide the three components of the magnetic field on the two-dimensional photospheric surface as boundary conditions.

Previously, we introduced a novel method for reconstructing coronal magnetic fields based on the poloidal-toroidal (PT) representation, which led to the development of the NFPT (Nonvariational Force-Free Field Code in Poloidal-Toroidal Formulation) in Cartesian coordinates. However, this approach did not account for the spherical geometry of the Sun's surface.

In this study, we present an improved FFF code that operates in spherical coordinates, incorporating the PT representation. This approach facilitates straightforward implementation of photospheric boundary conditions, with vector magnetogram data used as input. In our code, the source-surface top boundary is set at 2.5 solar radii, where the source surface region is believed to exist. The new code has been validated against analytic models by Low and Lou (1990) and compared with other FFF codes. This spherical-coordinate-based code aims to improve the accuracy of magnetic field information in an equilibrium state, thereby bringing qualitative enhancements to the initial conditions for global heliospheric modeling.

How to cite: Yi, S., Choe, G.-S., Kim, S., and Lee, M.: A Novel Poloidal-Toroidal Approach for Spherical Force-Free Field Reconstruction of Coronal Magnetic Fields, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3962, https://doi.org/10.5194/egusphere-egu25-3962, 2025.

We explored the origin of quasi-periodic pulsations (QPPs) in multiple wavelengths of a white-light flare, which occurred at the edge of a sunspot group. A short period at about 3 minutes is simultaneously observed in wavebands of HXR, microwave, and Lyα during the flare impulsive phase. The onset of flare QPPs is almost simultaneous with the start of magnetic cancellation between positive and negative fields, indicating that it is most likely triggered by accelerated electrons that are associated with periodic magnetic reconnections. A long period at about 8 minutes is only detected in the white-light emission, suggesting the presence of cutoff frequency. The similar periods of 3 and 8 minutes are measured at the umbra and penumbra in the adjacent sunspot. Moreover, the NLFFF extrapolation results suggest that the flare area and sunspots are connected by the magnetic field lines. Our observations support the scenario that the short-period QPP is modulated by the slow magnetoacoustic wave originating from the sunspot umbra, while the long-period QPP is probably modulated by the slow-mode magnetoacoustic gravity wave leaking from the sunspot penumbra.

How to cite: Li, D.: Exploring the origin of quasi-periodic pulsations during a white-light flare, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3997, https://doi.org/10.5194/egusphere-egu25-3997, 2025.

EGU25-4616 | ECS | Posters on site | ST1.7

Kinetic-Hybrid Simulations of Counter-Propagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind 

Yifan Wu, Chen Shi, Jinsong Zhao, and Xin Tao

Ion cyclotron waves (ICWs) are prevalent in the near-Sun solar wind and play a significant role in the nonadiabatic heating of plasma. Recent observations from the Parker Solar Probe (PSP) have revealed the simultaneous presence of anti-sunward and sunward ICWs in the vicinity of the Alfvén surface. However, single-satellite observations cannot effectively trace the generation and evolution of these observed waves. To address this limitation, we employ kinetic-hybrid simulations to replicate the generation and evolution of counter-propagating ICWs under typical plasma conditions in the near-Sun solar wind. Following the linear growth phase, the simulated waves exhibit amplitude and polarization characteristics that closely match the observations. Additionally, our simulation illustrates proton scattering and helium heating induced by the counter-propagating waves. These results underscore the significance of locally generated ICWs in influencing solar wind ion dynamics.

How to cite: Wu, Y., Shi, C., Zhao, J., and Tao, X.: Kinetic-Hybrid Simulations of Counter-Propagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4616, https://doi.org/10.5194/egusphere-egu25-4616, 2025.

EGU25-5369 | Orals | ST1.7

A  Simulation of Energy Exchange from Magnetotail Reconnection to the Inner Magnetosphere 

Raymond Walker and Liutauras Rusiatis

We have used a particle-in-Cell (PIC) simulation combined with a global MHD simulation to investigate energy transport from reconnection in the magnetotail to the inner magnetosphere. Initially, we ran an MHD simulation driven by nominal solar wind parameters and southward IMF. After reconnection starts in the magnetotail, we loaded the PIC simulation with plasma based on the MHD parameters. The PIC simulation extended from the solar wind outside of the bow shock to beyond the reconnection region in the tail and was run for 1m 47s. During that time, particles from the reconnection region reached the inner magnetosphere. We evaluated the transport of energy by examining the ion and electron energy fluxes, the Poynting flux and the changes in the particle and electromagnetic power densities in the simulation box as functions of time. We evaluated the changes in the energy densities by examining the divergences of the ion and electron energy fluxes and the Poynting flux. The particles move earthward in narrow channels like bursty-bulk-flows (BBFs). The Poynting power density is smaller than the ion particle power density. The ion kinetic power density is larger than the thermal power density. The energy exchange between kinetic energy and thermal energy is determined by the off-diagonal terms in the pressure tensor.

 

How to cite: Walker, R. and Rusiatis, L.: A  Simulation of Energy Exchange from Magnetotail Reconnection to the Inner Magnetosphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5369, https://doi.org/10.5194/egusphere-egu25-5369, 2025.

EGU25-5598 | Orals | ST1.7 | Highlight

Three-Dimensional Magnetohydrodynamic (MHD) Modeling of Solar Wind Near Mars by Combinng with data assimilation method 

Fang Shen, Hanke Zhang, Yi Yang, Yutian Chi, Chenglong Shen, and Xinyi Tao

Combined with data assimilation methods, a three-dimensional magnetohydrodynamic (MHD) numerical model is an effective tool to explore the mechanism of space weather. As a driver of space weather, the dynamic development of stream interaction regions (SIRs) near the orbit of Mars is an area of active research. In this study, we use the interplanetary total variation diminishing (TVD) MHD model to simulate solar wind parameters and
model SIRs near Mars from 2021 November 15 to 2021 December 31. In this model, the MHD equations are solved by the conservation TVD Lax–Friedrichs scheme in a rotating spherical coordinate system with six component meshes used on the spherical shell. Solar wind velocity, density, temperature, and magnetic field strength are given at the inner boundary due to the characteristic waves propagating outward. We compared modeled results with observations from Mars Atmospheric Volatile EvolutioN (MAVEN) and Tianwen-1 (China’s first Mars exploration mission). Statistical analysis shows that the simulated results can capture SIRs and are in good agreement with observations; moreover, the assimilated results based on the Kalman filter improve the accuracy of numerical prediction compared with simulated results. This paper is the first attempt to simulate SIR events combined with MAVEN and Tianwen-1 in situ observations. Our work demonstrates that using the MHD model with the Kalman filter to reconstruct solar wind parameters can help us study the characteristics of SIRs near Mars, improve the capabilities of space weather forecasting, and understand the background solar wind environment.

How to cite: Shen, F., Zhang, H., Yang, Y., Chi, Y., Shen, C., and Tao, X.: Three-Dimensional Magnetohydrodynamic (MHD) Modeling of Solar Wind Near Mars by Combinng with data assimilation method, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5598, https://doi.org/10.5194/egusphere-egu25-5598, 2025.

EGU25-6157 | Posters on site | ST1.7

Coherent Wave Excitation by Energetic Ring-beam Electrons in Inhomogeneous Solar Corona 

Xiaowei Zhou, Patricio Munoz, Jan Benacek, Lijie Zhang, Dejin Wu, Ling Chen, Zongjun Ning, and Joerg Buechner

Coherent radio emission mechanism of solar radio bursts is one of the most complicated and controversial topics in the solar physics. To clarify mechanism of different types of solar radio bursts, (radio) wave excitation by energetic electrons in homogeneous plasmas has been widely studied via particle-in-cell (PIC) code numerical simulations. In this study, we, however, investigate effects of inhomogeneity in plasmas of the solar coronal on wave excitation by ring-beam distributed energetic electrons utilizing 2.5-dimensional PIC simulations. Disequilibrium introduced by the inhomogeneous magnetic field is balanced by either inhomogeneous density or inhomogeneous temperature of the background plasma. Both the beam and electron cyclotron maser (ECM) instabilities could be triggered with the presence of the energetic ring-beam electrons. Onset of the ECM instability is, however, later than the beam instability to excite waves in this study. The resultant spectrum of the excited electromagnetic waves presents a zebra-stripe pattern in the frequency space. The inhomogeneous density or temperature in plasmas would, however, influence the frequency bandwidth, excitation location of these excited waves. This study will, hence, help diagnose the plasma properties at the generation sites of solar radio bursts. Applications of this study to solar radio bursts (e.g., solar type V, zebra-pattern radio burst) will be discussed.

How to cite: Zhou, X., Munoz, P., Benacek, J., Zhang, L., Wu, D., Chen, L., Ning, Z., and Buechner, J.: Coherent Wave Excitation by Energetic Ring-beam Electrons in Inhomogeneous Solar Corona, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6157, https://doi.org/10.5194/egusphere-egu25-6157, 2025.

EGU25-6853 | Posters on site | ST1.7

Self-consistently generated, evolving and propagating interplanetary shocks with 3D hybrid simulations 

Emanuele Cazzola, Dominique Fontaine, and Philippe Savoini

Interplanetary shocks (IPs) are ubiquitous in the Heliosphere, and are particularly relevant when associated to Stream Interaction Regions and Coronal Mass Ejections due to their great geomagnetic effectiveness on Earth. As their evolution and propagation may vary based on the different interplanetary conditions, it is crucial to study the shocks characteristics under different scenarios to gain a better understanding of the different types of interactions with the near-Earth environment.  

In this work, we propose a systematic analysis of the evolution, propagation and characterization of self-consistently generated interplanetary shocks under different conditions, such as different interplanetary magnetic field intensity, direction and particles density, velocity, by means of hybrid computer simulations (fluid electrons, kinetic ions).  The use of a hybrid formalism allows us to simulate large domains necessary for the shocks to form and evolve, by still retaining the kinetic information, which is fundamental to consider important kinetic effects, e.g., in supercritical shock-fronts. 

In particular, upon setting up an initial steepening velocity profile between slower and faster velocities, we observe this profile to evolve in a two boundaries-structure, separated by a turbulent sheath.  We first qualify these boundaries relative to the structure expected from steady shocks, we estimate their respective velocity and their compression factor. We also analyse the main characteristics of the turbulent sheath, which propages at an intermediate velocity with a enhanced magnetic field and transverse components in the magnetic field and velocity. All these features are consistent with observations of SIRs at 1 AU (e.g., Jian+, 2006). Moreover, we also discuss the effects of different IMF orientations on the shock dynamics, as the different kinetic effects between a quasi-perpendicular and quasi-parallel configuration at the shock can bring to significant differences in the shock-front propagation and the related donwstream sheath turbulence.

How to cite: Cazzola, E., Fontaine, D., and Savoini, P.: Self-consistently generated, evolving and propagating interplanetary shocks with 3D hybrid simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6853, https://doi.org/10.5194/egusphere-egu25-6853, 2025.

EGU25-8769 | ECS | Posters on site | ST1.7

Beam-driven evaporation in 2.5D flare simulations with an asymmetric magnetic field configuration 

Maxime Dubart, Malcolm Druett, and Rony Keppens

The standard flare model is in generally depicted and studied in 2D simulations with an anti-symmetrical magnetic field configuration, symmetrical in magnitude, either side of the polarity inversion line. However, flare observations confirm that most flare have a significantly asymmetrical values of the magnetic field strength. 

Here we present the first multi-dimensional magnetohydrodynamic flare simulation featuring evaporation driven by energetic electron beams in an asymmetrical magnetic field configuration. The simulation conditions that we use are known to rely significantly on those beams of electrons to drive the evaporated plasma upwards from the lower atmosphere (Druett et al. 2023). We study the impact of an asymmetrical configuration on the evolution and geometry of the flare-loop system as well as the impacts on the beam-driven evaporation using the MPI-AMRVAC model.

This results in multiple Hard X-Rays deposition sites in the lower atmosphere, Hard X-Rays sources forming at the top of the flare loop, and a sustained rotating flux rope structure with associated footpoint electron deposition flux.

How to cite: Dubart, M., Druett, M., and Keppens, R.: Beam-driven evaporation in 2.5D flare simulations with an asymmetric magnetic field configuration, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8769, https://doi.org/10.5194/egusphere-egu25-8769, 2025.

EGU25-11264 | ECS | Posters on site | ST1.7

Adaptive mesh and model refinement for numerical plasma models 

Ulysse Caromel, Nicolas Aunai, Roch Smets, and Philip Deegan

The next generation of numerical plasma models need to have the capacity to address multi-scale problems for which fluid-only codes miss physics and pure kinetic codes are too computationally heavy. The code PHARE, currently being developed, aims at enabling the evolution of complex plasma systems over a dynamic hierarchy of grids with different mesh resolutions and potentially different plasma formalisms as well. This Adaptive Mesh and Model Refinement (AM2R) will provide better resolution and better realism to the solution where and when assessed necessary. This work will present the ongoing progress on the project, regarding the AMR Hybrid-PIC and AMR Hall-MHD solvers.

How to cite: Caromel, U., Aunai, N., Smets, R., and Deegan, P.: Adaptive mesh and model refinement for numerical plasma models, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11264, https://doi.org/10.5194/egusphere-egu25-11264, 2025.

EGU25-13772 | ECS | Posters on site | ST1.7

Kinetic Effects of Rotational Discontinuities on Maxwellian and Non-Maxwellian plasmas 

Rong Lin, Fabio Bacchini, and Jiansen He

Rotational discontinuities (RDs) are considered in magnetohydrodynamics (MHD) as a kind of stable, persistent structure. As recent observations have shown, RDs may effectively describe the boundaries of switchbacks in the solar wind, around / inside which the plasma is highly dynamic and with phase space density variations. Because of the low collisionality of the solar wind, it may be worthwhile to revisit RDs with a kinetic approach. We therefore model the the plasma in RDs representing switchbacks with the state-of-the-art full-particle simulation code ECSim, and discuss the kinetic effects occurring in RD plasmas, including proton heating, anisotropy alternation, and modification of a core-beam composition, as well as the potential implications for the nature of switchbacks.

How to cite: Lin, R., Bacchini, F., and He, J.: Kinetic Effects of Rotational Discontinuities on Maxwellian and Non-Maxwellian plasmas, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13772, https://doi.org/10.5194/egusphere-egu25-13772, 2025.

In collisionless plasmas such as the solar wind, the particle velocity distributions can be shaped by various wave-particle interactions, which lead to effective energy transfer between electromagnetic fields and particles. The commonly-observed quasi-monochromic waves by in-situ satellites are widely believed to be generated by plasma instabilities via wave-particle interactions. Thus, how to quantify the role(s) of wave-particle interactions in plasma instabilities is a fundamental problem in the space plasma community. Recently, we developed a theoretical method quantifying both resonant and nonresonant wave-particle interactions, and we performed the comprehensive analyses on ion temperature anisotropy instabilities in the solar wind. This report will introduce new findings.

How to cite: Zhao, J.: Quantifying wave-particle interactions in ion temperature anisotropy instabilities, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13988, https://doi.org/10.5194/egusphere-egu25-13988, 2025.

Modeling Solar magnetic field in the corona is very important to understand the solar eruption and heating mechanism. However, the direct measurements of solar magnetic field in the solar corona is still taking a great challenge not only in the high accurate measurements of solar polarization signal, but also in the inversion approach for the Optic-thin condition of corona atmosphere. Existence and uniqueness in the force-free/Non-force-free extrapolation in the solar corona is still unknown. Magnetic helicity, as a topological invariant, has become a key factor in exploring the generation of magnetic fields within the Sun, solar eruptions, and energy transfer processes in interplanetary. We firstly give a short review of modelling magnetic helicity in the solar corona from the observation to simulation. Then we introduce a new method by calculating the potential current in a magnetic-helicity-conservation-decomposed approach to derive the magnetic helicity/energy equivalence of three-dimension magnetic field only based on the photospheric vector magnetogram. We testify our method by using the given magnetic field of Low and Lou (1990) and the difference is very small. Even though, the Lorentz force caused from the calculated magnetic field well explained the strong shearing movements of polarity inversion line (PIL) in the newly emerging active region of NOAA11158. Finally, we apply our method to the observation data and it is also successfully found that the weak/strong loss ratio of magnetic helicity in the solar confined/eruptive solar events.

How to cite: Yang, S.: Modeling Solar Magnetic Field In The Solar Corona From The View Of Magnetic Helicity, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14276, https://doi.org/10.5194/egusphere-egu25-14276, 2025.

EGU25-16188 | Orals | ST1.7

Open SESAME: status and further plans 

Stefaan Poedts and the Open SESAME

The ERC-AdG project Open SESAME (project No 101141362) aims to develop a time-evolving model for the entire solar atmosphere, including the chromosphere and transition region, based on a multifluid description. Currently, models are primarily steady, rely on a single-fluid description and include only the corona due to computational challenges. We plan to use time-evolving ion-neutral and ion-neutral-electron models. The multifluid approach will enable us to describe the intricate physics in the partially ionised chromosphere and quantify the transfer of momentum and energy between the atmospheric layers. The questions of where the solar wind originates and solar flares and coronal mass ejections are driven have fundamental scientific importance and substantial socio-economic impact. Indeed, the solar atmospheric model is the crucial missing link in the Sun-to-Earth model chain to predict the arrival and effects of CMEs on Earth.

This goal is now possible by combining our implicit numerical solver with a high-order flux-reconstruction (FR) method. The implicit solver avoids the numerical instabilities that lead to strict time-step limitations on explicit schemes. The high-order FR method enables high-fidelity simulations on very coarse grids, even in zones of high gradients. We started with this new development and will introduce three critical innovations. First, we will combine high-order FR with physics-based r-adaptive (moving) unstructured grids, redistributing grid points to regions with high gradients. Second, we will implement CPU-GPU algorithms for the new heterogeneous supercomputers advanced by HPC-Europa. Third, we will implement AI-generated magnetograms to make the model respond to the time-varying photospheric magnetic field, which is crucial for understanding important solar plasma properties and processes.

Thus, we will develop a first-in-its-kind high-order GPU-enabled 3D time-accurate solver for multifluid plasmas. If successful, we will implement the most advanced data-driven solar atmosphere model in an operational environment. The project started on 1 September 2024, and we already have interesting results on time-dependent corona modelling and high-order flux-reconstruction simulations.

How to cite: Poedts, S. and the Open SESAME: Open SESAME: status and further plans, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16188, https://doi.org/10.5194/egusphere-egu25-16188, 2025.

We report an M9.3 flare and filaments activities from NOAA Active Region 11261 that are strongly modulated by the 3D magnetic skeleton. Magnetic field extrapolation from the vector magnetic field suggests complex magnetic connectivity and the existence of a high coronal null point southeast of the active region. A small filament over the  inversed V-shaped polarity inversion line erupted and resulted in the M9.3 flare associated with a weak hot mass ejection, CME-like features, and the formation and activity of a relatively large filament. The ejection features and the eruption of the large filament were toward the southeast. Comparative analyses have disclosed the following new facts: (1) the trajectory of looptop hard X-ray emission provides solid evidence that the magnetic reconnection site propagated up toward the coronal null point as the flare and filaments erupted. (2) the EVU observations show coronal mass ejection-like eruption features in the ejection region of the magnetic skeleton. (3) the closed fan confined the west end of the large filament and the corresponding flare ribbons. We demonstrate a spatiotemporal relationship between the magnetic skeleton and the flare filament activity. We conclude that the magnetic skeleton can modulate and determine almost all the characteristics of the studied activity in the corresponding scale.

How to cite: Guo, J.: The Role of Magnetic Skeleton in Solar Flare Filaments Activities, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16745, https://doi.org/10.5194/egusphere-egu25-16745, 2025.

The solar wind is an accessible natural laboratory for investigating thermal and energetic particles in space plasmas. The particle dynamics in the solar wind has a highly multi-scale nature, covering 8 orders of magnitude of spatial scales, from the lengths characteristic of the electron gyromotion around magnetic field lines ( ~1 km) to those characteristic of particle transport from the Sun to the Earth ( ~ 1 au). Studying such dynamics is a difficult endeavour, especially due to the solar wind’s strongly turbulent nature. Current models of particle dynamics in turbulent plasmas suffer from one or more limitations, such as unrealistic plasma background (e.g., 2D modelling, lack of the correct statistical turbulent properties such as anisotropy and intermittency of structures) or limited accuracy (e.g., small computational grids, low resolution in phase space). Most importantly, they only employ one simulation at a time and thus they only model the turbulent energy cascade over three decades of scales at best. 
We present our innovative solution to overcome all those limitations: the multi-scale Box-in-Box (BIB) approach.  The first step is to model the turbulent energy cascade from very large to very small scales, using a portion of a large simulation as initial condition for another one with higher resolution and repeating this process multiple times in sequence while coupling different physical models, e.g., MHD at the largest scales, hybrid across the ion scales, and fully kinetic at electron ones. The second step is advancing test-particles trajectories using the turbulence simulations as an evolving background from small to large scales, starting from the fully kinetic simulation and then switching to the hybrid and finally to the MHD one as the energy (and thus the gyroradius) of the test particles increases. We will show and discuss the main technical challenges of this kind of approach, the required operations in the different steps of the procedure, and some successful results. Our innovative BIB approach makes it possible to model the large-scale propagation of energetic particles in the turbulent solar wind while retaining a realistic and self-consistent description of the microphysics responsible for particle energization. Our BIB simulations will be particularly useful for developing and testing new visualisation and analysis techniques for future multi-scale space missions such as HelioSwarm and Plasma Observatory.

How to cite: Franci, L., Papini, E., and Trotta, D.: Modelling the particle dynamics in turbulent plasmas using the innovative multi-scale Box-In-Box (BIB) approach, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19152, https://doi.org/10.5194/egusphere-egu25-19152, 2025.

EGU25-21910 | ECS | Orals | ST1.7

CMEs and Interplanetary Shocks: 2.5D Numerical Modeling 

Xiaozhou Zhao

Solar flares, eruptive prominences (EPs), and coronal mass ejections (CMEs) significantly impact Earth's environment and human habitability, as they are different manifestations of solar storms. Sometimes, solar energetic particle events (SEPs) are associated with interplanetary shocks driven by CMEs that propagate through the turbulent solar wind. We investigate the physical mechanisms of these phenomena in a more realistic gravitationally stratified solar atmosphere using 2.5D magnetohydrodynamics (MHD) and particle simulations. Our research covers three main topics:

(1) MHD simulations of solar flux rope eruptions and prominence formation: Starting from the standard solar eruption model, we employed 2.5D MHD simulations to investigate two scenarios of flux rope and prominence eruptions within a more realistic, gravitationally stratified solar atmosphere. We developed an enhanced levitation model for prominence formation and proposed a novel mechanism involving plasmoid-fed processes in the current sheet. The former is driven by photospheric converging motions, while the latter focuses on the catastrophe model of flux rope eruption and emphasizes the crucial role of magnetic reconnection in prominence formation. These models describe the formation of flux ropes during eruption and pre-existing flux ropes beforehand, respectively. Additionally, we explored "mesoscale" phenomena during flux rope eruption and their association with Quasi-Periodic Pulsations (QPPs), reproducing multi-wavelength observational images.

(2) Shock-turbulence interactions in interplanetary space: Solar wind turbulence is ubiquitous, and when CMEs propagate through the solar wind, they drive interplanetary shocks that interact with solar wind turbulence, which is one of the sources of SEPs. These interactions result in a turbulent downstream fluid. We found that after shocks propagate across turbulence, the downstream occurrence of plasmoids (i.e., small magnetic flux ropes in the solar wind) increases, saturates to a peak value for a certain interval, and then gradually decreases away from the shock. This behavior is consistent with in-situ measurements taken by the Magnetospheric Multiscale (MMS) mission at Earth's bow shocks. These plasmoid structures are important for plasma heating and particle acceleration.

(3) Particle accelerations during solar eruptions: We investigated particle acceleration during solar eruptions, focusing on: 1) test-particle modeling of non-adiabatic motion of particles in 2D magnetic islands and 2) a combined Particle-In-Cell (PIC) and MHD approach (PIC-MHD) to study particle acceleration at interplanetary shocks. In the PIC-MHD approach, the background thermal plasma is treated as a magnetofluid, while the motion of non-thermal particles is influenced by the Lorentz force. This method accounts for electromagnetic interactions between non-thermal particles and the background magnetofluid, potentially leading to upstream self-excited turbulence that enhances particle acceleration through various mechanisms.

Overall, our research focuses on various processes in solar storms. Understanding and even predicting these phenomena are crucial for studying their impact on human habitability.

How to cite: Zhao, X.: CMEs and Interplanetary Shocks: 2.5D Numerical Modeling, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21910, https://doi.org/10.5194/egusphere-egu25-21910, 2025.

Ellerman bombs (EBs) and ultraviolet (UV) bursts are two of the smallest observed solar activities triggered by magnetic reconnection in the lower solar atmosphere, typically associated with flux emergence regions. Joint observations from the Interface Region Imaging Spectrograph (IRIS) satellite and ground-based solar telescopes reveal that approximately 20% of hot UV bursts are temporally and spatially connected with the cooler EBs. Using 3D radiation magnetohydrodynamic (RMHD) simulations with the MURaM code, we investigated the spontaneous emergence of a magnetic flux sheet, leading to complex magnetic field structures and diverse high-temperature activities due to magnetic reconnection. The simulations show that opposite-polarity magnetic fields converge in the lower solar atmosphere, forming thin current sheets and triggering plasmoid instability, which results in small twisted magnetic flux ropes and highly nonuniform plasma density and temperature. Hot plasmas (>20,000 K) emitting strong UV radiation coexist with cooler plasmas (<10,000 K) showing Hα wing emissions, with the former located ~700 km above the solar surface and the latter above them. Synthesized images and spectral line profiles exhibit characteristics of both EBs and UV bursts, demonstrating that turbulent reconnection mediated by plasmoid instability can occur in small-scale reconnection events in the partially ionized lower solar atmosphere. This model explains the formation mechanisms of UV bursts connected with EBs and indicates that UV bursts can form in atmospheric layers extending from the lower chromosphere to the transition region.

How to cite: Cheng, G.: Turbulent Reconnection in the Lower Solar Atmosphere Triggers UV Bursts Connecting with Ellerman Bombs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21916, https://doi.org/10.5194/egusphere-egu25-21916, 2025.

NP7 – Nonlinear Waves

Compared to 2-way coupled simulations over the Gulf of Mexico (GOM), additional wave (3-way) coupling shifts the energy of the surface flow toward the model grid resolution (8-9 km) and showed  higher energy in the velocity potential component than the divergence component. The heat budget of the Loop Current showed differences  between 2- and 3-way coupling. e.g. the magnitude of the heat tendency and the pattern of the advection term. and also a strong TC quadrant-dependent heat budget when a TC interacts with the LC. For instance, the heat budget at the LC warm core and at a TC center was ~1.5 times smaller for 3-way coupling than the 2-way counterpart. On the other hand, the heat at the LC front and TC right-quadrant were about the same magnitude regardless of coupling, but the large negative trend for 3-way coupling at the time a TC passed was not completely accounted for by the individual budget terms. It is interesting to observe a shift from the rotational field dominant for a pre-storm period to the divergence component during the TC passage, which might be related to the storm-induced upwelling. 

 

How to cite: Kim, H.-S. and Shao, M.: Numerical investigation of 3-way coupled tropical cyclone (TC)-Loop Current (LC)-wave non-linear interactions, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1260, https://doi.org/10.5194/egusphere-egu25-1260, 2025.

EGU25-2505 | Orals | OS1.10

Numerical-analytical solutions to mud mechanical responses to the waves in shallow water regions: From cohesive sediment to fluid mud 

Sarmad Ghader, S. Hadi Shamsnia, Henrik Kalisch, Jan Nordström, and S. Abbas Haghshenas

 Abstract:

A comprehensive overview to the mud liquefaction and fluid mud mass transport induced by waves and currents are proposed in the shallow water regions. In this regard, the Shallow Water Equations (SWEs) must be solved for the upper water layer and the mud mechanical response to the free surface must be investigated. The aim of the present study, thus, is two folded: 1) To numerically investigate the newly developed energy-stable skew-symmetric form of the linear and nonlinear shallow water equations (SWE) using high-order numerical schemes with the so-called summation by parts (SBP) property; 2) analytical solutions to the interactions between waves, currents, and the muddy bed layer and compare the results for different constant, linear, and second-order current profiles.

The nonlinear stable boundary treatments with penalty-like simultaneous approximation terms (SAT), have been applied to mimic the lifting approach of continuous characteristic boundary conditions. In order to test the skew-symmetric form of SWE with the new variables, a manufactured solution (MS) is deployed, and the scheme is shown to be robust in the domain and at the boundary sides. The free parameters in the new form of the equations slightly change the convergence.

The effects of mean shear stress and its variations on wave dispersion relations as well as mud (particle and mass transport) velocities are investigated. It is found that the second-order profile presents the maximum effects on the wave field (wave dissipation and mud mass transport velocities) compared to the constant and linear current profiles. However, assuming the constant current profile, frequently applied in the literature models, results in the minimum effects. A local peak exists in the mud mean discharge over the current profile curvature. The mud velocity induced by the linear current profile presents the closest value to the particle velocity for the no-current case. Additionally, the second-order current profile provides slightly better results for the mud mass transport velocity rather than the constant current profile when comparing the results with the laboratory data.

There is a rather huge gap between the existing agreed mechanisms in the literature for non-cohesive and cohesive sediment which is addressed. Also, the lack of experimental and theoretical results for the mud liquefaction mechanism is pointed out. Open questions in the field and potential topics for further research are presented.

Keywords:

Shallow water equations, Mud mass transport, Wave-current-mud interaction, Summation by parts, Stable boundary conditions, Mud liquefaction and transport

How to cite: Ghader, S., Shamsnia, S. H., Kalisch, H., Nordström, J., and Haghshenas, S. A.: Numerical-analytical solutions to mud mechanical responses to the waves in shallow water regions: From cohesive sediment to fluid mud, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2505, https://doi.org/10.5194/egusphere-egu25-2505, 2025.

EGU25-3850 | Orals | OS1.10

Sea ice break-up potential by locally generated wind waves in a polynya 

Joey Voermans, Qingxiang Liu, Lang Cao, Petra Heil, Clarence O. Collins, Josh Kousal, Jean Rabault, and Alexander Babanin

Polynyas, regions of open water enclosed by sea ice, are persistent features near the Antarctic coast as well as in the pack ice. Waves are known to occur within polynyas. If a polynya is sufficiently separated from the “blue” Southern Ocean by pack ice, then it can be considered isolated from Southern Ocean waves. Wave energy in isolated polynyas must be generated locally. During offshore wind conditions, a polynya could provide a long fetch for waves to develop, and the wind-waves may be steep enough to break the ice pack from the inside outward. This is in contrast to the typical focus of wave-induced sea ice break-up from the outside-inward with waves originating from the Southern Ocean. Here, we present our investigation of this inside-out sea-ice erosion mechanism based on buoy measurements of waves in the Vincennes Bay Polynya, East Antarctica. The measurements confirm the presence of energetic locally generated waves, which appear to be sufficiently steep to break the ice at the polynya edge. Further, we evaluate the wave-induced sea-ice break-up potential in this recurring polynya over the past two decades. Our results confirm the importance of locally generated waves in Antarctic polynyas. This highlights the previously overlooked potential of waves to accelerate sea-ice loss from within the pack ice, contributing to the recent Antarctic sea-ice decline.

How to cite: Voermans, J., Liu, Q., Cao, L., Heil, P., Collins, C. O., Kousal, J., Rabault, J., and Babanin, A.: Sea ice break-up potential by locally generated wind waves in a polynya, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3850, https://doi.org/10.5194/egusphere-egu25-3850, 2025.

Submesoscale processes usually have characteristic horizontal scales of O(0.1 to 10) km and timescales of O(0.1 to 10) days, and play significant roles in energy cascade and vertical tracer transport which affect ocean circulation, air-sea interactions, and biogeochemical cycles. As an effective way, high-resolution simulations have been conducted to study submesoscales. The hydrostatic approximation becomes unsuitable for high-resolution ocean modeling because the horizontal scales of the motions are comparable to the local vertical scales. Combining hydrostatic and non-hydrostatic pressure in the ocean general circulation models (OGCMs) contributes to accurate modeling. Based on the pressure correction method, the non-hydrostatic dynamics are implemented into the hydrostatic OGCM. Based on the numerical simulation, the dynamic characteristics and spatiotemporal Variations of submesoscales in the South China Sea (SCS) are analyzed, and two leading generation mechanisms, including strain-induced frontogenesis and mixed layer baroclinic instabilities, are discussed through the vertical buoyancy transport and potential vorticity budget analysis. The comparison also shows that the simulated internal tide signature by non-hydrostatic OGCM is more obvious, and the simulated temperature are significantly closer to the Argo data. The construction of non-hydrostatic OGCM greatly promotes high-resolution ocean modeling and is of great significance for the research on the multi-scale interaction.

How to cite: Zhuang, Z.: A numerical study of submesoscale dynamic processes in the Northern South China Sea, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3878, https://doi.org/10.5194/egusphere-egu25-3878, 2025.

EGU25-6011 | Posters on site | OS1.10

Reconstruction of directional wind wave spectra from visual ship-based observations 

Vika Grigorieva, Vitali Sharmar, Sergey Gulev, and Yaron Toledo

For the first time, directional wave spectra are reconstructed from visually observed wind wave data over the North Atlantic Ocean. For this purpose, a novel analytical approach for calculating the directional spreading function from visual ship-based observations is proposed. Natively and inherently separated estimates of wind sea and swell heights, periods, and directions of propagation provide independent directional spreading functions for wave systems in a given area and time. Shape parameter and the mean angle are evaluated from spatially and temporally averaged sine and cosine projections of wave directions. The calculated directional spreading functions combined with frequency spectra of wind sea and swell allow for two-dimensional spectra reconstruction from visible wave elements on different temporal and spatial scales. The new approach was applied to visual wave observations in the North Atlantic for the period of 1970-2023. Visual wave observations were taken from the ICOADS (International Comprehensive Ocean-Atmosphere Data Set), consolidating all available observations by Voluntary Observing Ships (VOS). Directional wave spectra were reconstructed in two spatial grids: 10°x10° and 1°x1° with a temporal resolution varied from one day to climatological month. The results were intercompared to the directional spectra derived from the long-term model hindcasts of wind waves performed with WWIII spectral wave model for both individual daily spectra and regional spectral climatology of wind waves. We also analyzed interdecadal changes of directional spectra in both VOS-based and model products and their ability to explain observed and modeled changes in wind wave heights and directions. Thus, the ability to derive directional wave spectra from visual observations adds a new value to the conventional analysis of wind sea and swell systems in terms of heights and periods.

How to cite: Grigorieva, V., Sharmar, V., Gulev, S., and Toledo, Y.: Reconstruction of directional wind wave spectra from visual ship-based observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6011, https://doi.org/10.5194/egusphere-egu25-6011, 2025.

EGU25-6161 | ECS | Orals | OS1.10

Resonant Triad Interactions of Acoustic and Gravity Waves in Water of Finite Depth 

Emanuele Zuccoli and Usama Kadri

The interaction between acoustic and surface-gravity waves is typically disregarded in classical wave theory due to their distinct propagation speeds. However, nonlinear dynamics enable energy exchange through resonant triad interactions, facilitating significant coupling between these wave types. This study investigates the resonant interaction involving two acoustic modes and one gravity wave in water of finite and deep depths. Using the method of multiple scales, nonlinear amplitude equations are derived to characterise the system’s spatio-temporal behaviour.

The analysis reveals that energy transfer efficiency depends strongly on water depth. While deeper water hinders energy transfer, shallower regimes enhance interaction, particularly when higher acoustic modes are involved. Numerical simulations identify parameter ranges where gravity wave amplitudes can be amplified or reduced, contingent on factors such as initial acoustic amplitudes and wave packet widths.

These findings have implications for tsunami mitigation, offering a potential mechanism to reduce wave amplitudes before reaching shorelines. Furthermore, the insights contribute to renewable energy harnessing from surface gravity waves by leveraging resonant acoustic-gravity interactions. This work advances the theoretical framework for understanding acoustic-gravity wave dynamics, highlighting opportunities for practical applications in environmental and energy contexts.

How to cite: Zuccoli, E. and Kadri, U.: Resonant Triad Interactions of Acoustic and Gravity Waves in Water of Finite Depth, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6161, https://doi.org/10.5194/egusphere-egu25-6161, 2025.

EGU25-8089 | Posters on site | OS1.10 | Highlight

Wave Growth at Low Atmospheric Pressure 

Alexander Babanin, Eduardo Palenque, Joey Voermans, Christian Lopez, and Andrei Babanin

The Titicaca project is intended to experimentally test theoretical and empirical models used in fluid mechanics to describe wind-wave interactions. At Lake Titicaca, which is located at altitude of 3800 m, atmospheric pressure is reduced to some 60% by comparison with the sea level. Titicaca, with deep waters in excess of 250 m, has an elongated shape with the long axis of120 km and its short axis of 50 km, and provides wave fetches which are long enough for wave development across a full range of sea state conditions

All modern wave models are validated considering data at the sea level. In the theory, air density and pressure are variable, but in experiments at the sea level they are not. Therefore, the study, apart from academic merits, also has practical value in practical terms of wave forecast. For example, significant change of air pressure is not uncommon (e.g. up to 20%) in tropical cyclones, which fact can lead to respective, or larger errors for predicted wave heights, but so far is not accounted for.

The objective of the project is to measure wave generation, development and breaking in conditions of low air density and air pressure. Standard non-dimensional dependences for wave evolution (normalized by the local wind) are investigated and compared to the known (sea level) results. Evolution of the wave spectrum under the low-pressure winds is studied and benchmarked against classic JONSWAP development of wind-generated waves.

As expected, evolution of waves forced by the wind under low pressure is different to the sea level, but details of the differences are not necessarily expected. For the same wind forcing, Titicaca waves start with lower energy by comparison with their sea-level counterparts, but grow faster and catch up in magnitude towards the Pierson-Moscowitz conditions. Their spectrum exhibits higher levels of both enhancement and the tail towards full development, and we argue that it is stronger nonlinear fluxes across the spectrum that are responsible for faster growth of peak waves under weaker wind input at the tail. Comparison of low-pressure tropical-cyclone waves with the Titicaca evolution is conducted and demonstrate consistent behaviours.

How to cite: Babanin, A., Palenque, E., Voermans, J., Lopez, C., and Babanin, A.: Wave Growth at Low Atmospheric Pressure, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8089, https://doi.org/10.5194/egusphere-egu25-8089, 2025.

EGU25-9710 | Orals | OS1.10 | Highlight

ICON-waves: a new ocean surface waves component of the ICON modeling framework. 

Mikhail Dobrynin, Daniel Reinert, Heinz Günther, Florian Prill, Oliver Sievers, Vanessa Fundel, Panagiotis Adamidis, Arno Behrens, Thomas Bruns, and Günther Zängl
We present ICON-waves, a new component of the ICOsahedral Non-hydrostatic (ICON) modeling system, designed to explicitly model ocean surface gravity waves and their feedbacks on the atmosphere and ocean within the Earth system. Until now, the ICON-NWP model, developed and routinely operated by the German Weather Service (DWD), has not fully captured the impact of wave-induced interactions. Waves influence the sea surface state, generate turbulence, modify ocean currents, and affect air-sea exchanges of heat, matter, and momentum. ICON-waves addresses these processes by providing a wave-spectrum-dependent interface within the ICON framework, enabling more realistic simulations of atmosphere-ocean interactions. The integration of ICON-waves represents a significant advancement in modeling the complexity of atmosphere-ocean feedbacks, offering potential benefits for weather and climate prediction. This presentation outlines the ICON-waves model, including its concept, wave physics, and its role in improving overall model physics. We demonstrate results from both stand-alone ICON-waves and coupled ICON-NWP-waves simulations, focusing on the effects of wave-dependent sea surface roughness in the coupled atmosphere-waves system.

How to cite: Dobrynin, M., Reinert, D., Günther, H., Prill, F., Sievers, O., Fundel, V., Adamidis, P., Behrens, A., Bruns, T., and Zängl, G.: ICON-waves: a new ocean surface waves component of the ICON modeling framework., EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9710, https://doi.org/10.5194/egusphere-egu25-9710, 2025.

EGU25-11946 | ECS | Orals | OS1.10

Representing waves in ECMWF’s data-based forecasting system AIFS 

Sara Hahner, Jean Bidlot, Josh Kousal, Lorenzo Zampieri, and Matthew Chantry

Recent advancements in data-driven weather forecasting have demonstrated superior accuracy compared to traditional physics-based approaches for several components of the Earth system. While prior work on wave forecasting has focused on wave-atmosphere interactions through fine-tuning pre-trained models or training specific forced wave models, we present the results of training a joint model of waves and atmosphere, forecasting the two components simultaneously.

Surface winds, which can be well represented by data-driven atmospheric models, and waves are highly coupled. Therefore, we train a joint model of the atmosphere and waves, incorporating several wave fields into the deterministic Artificial Intelligence/Integrated Forecasting System (AIFS) at ECMWF [Lang et al., 2024]. For the training, a new dataset was constructed using ECMWF’s latest wave model [ECMWF, 2024; Yu et al., 2022]. The updated wave model offers an enhanced representation of wave fields especially under sea ice, resolving challenges with moving missing values.

The data-based wave forecasts are competitive with the ECMWF's operational physics-based wave model. Additionally, we present findings on how integrating wave fields enhances surface wind predictions. Through case studies, we illustrate the effectiveness of this approach, highlighting its potential to advance the accuracy and reliability of global weather forecasting systems.

 

[Lang et al., 2024] Simon Lang, Mihai Alexe, Matthew Chantry, Jesper Dramsch, Florian Pinault, Baudouin Raoult, Mariana C. A. Clare, Christian Lessig, Michael Maier-Gerber, Linus Magnusson, Zied Ben Bouallègue, Ana Prieto Nemesio, Peter D. Dueben, Andrew Brown, Florian Pappenberger, and Florence Rabier. AIFS – ECMWF’s data-driven forecasting system. arXiv preprint arXiv:2406.01465, 2024. https://arxiv.org/abs/2406.01465.

[ECMWF, 2024] IFS documentation CY49R1–Part VII: ECMWF wave model. ECMWF Tech. Rep. CY49R1, 120 pp.

[Yu et al., 2022] Jie Yu, W. Erick Rogers, and David W. Wang. A new method for parameterization of wave dissipation by sea ice. Cold Reg. Sci. Technol. 2022, 199, 103583.

How to cite: Hahner, S., Bidlot, J., Kousal, J., Zampieri, L., and Chantry, M.: Representing waves in ECMWF’s data-based forecasting system AIFS, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11946, https://doi.org/10.5194/egusphere-egu25-11946, 2025.

EGU25-11948 | Posters on site | OS1.10

Wave climate projections off coastal French Guiana based on high-resolution modelling over the Atlantic Ocean 

Ali Belmadani, Maurizio D’Anna, Léopold Védie, Déborah Idier, Rémi Thiéblemont, Philippe Palany, and François Longueville

Global warming is altering the atmosphere and ocean dynamics worldwide, including patterns in the generation and propagation of ocean waves, which are important drivers of coastal evolution, flood risk, and renewable energy, among others. In French Guiana (northern South America), where most of the population is concentrated in coastal areas, understanding future wave climate change is critical for regional development, planning and adaptation purposes. The most energetic waves typically occur in boreal winter, in the form of long-distance swell originating from the mid-latitude North Atlantic Ocean. However, existing high-resolution wave climate projections that cover the French Guiana region focus on the hurricane season only (summer-fall).

In this study, a state-of-the-art basin-scale spectral wave model and wind fields from a high-resolution atmospheric global climate model were used to simulate present and future winter (November to April) wave climate offshore of French Guiana. The model performance was evaluated against wave data from ERA5 reanalysis, satellite altimetry and coastal buoys between 1984 and 2013. A statistically significant overall projected decrease (~5 %) in wintertime average significant wave height and mean wave period was found for the 2051-2079 period under the RCP-8.5 greenhouse gas emission scenario, together with a ~1° clockwise rotation of mean wave direction and consistent reductions in extreme wave heights and frequency. The results suggest that these decreasing trends are primarily driven by changes in large-scale patterns across the Atlantic that counteract an expected increase in local wind speed. Such results are further discussed using the limited available data from a multi-model ensemble of global wave projections.

How to cite: Belmadani, A., D’Anna, M., Védie, L., Idier, D., Thiéblemont, R., Palany, P., and Longueville, F.: Wave climate projections off coastal French Guiana based on high-resolution modelling over the Atlantic Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11948, https://doi.org/10.5194/egusphere-egu25-11948, 2025.

EGU25-13092 | Posters on site | OS1.10

Directional wave spectrum retrieved from in-situ and remote sensors 

Francisco J. Ocampo-Torres, Pedro Osuna, Nicolas G. Rascle, Carlos F. Herrera Vázquez, Héctor García-Nava, Guillermo Díaz Méndez, Bernardo Esquivel Trava, Carlos E. Villarreal-Olavarrieta, and Rodney E. Mora-Escalante

Measurements of ocean surface waves are obtained and studied from various perspectives. A coastal high frequency radar and an acoustic Doppler current profiler have been deployed and operated to detect and determine the source of differences of wave information retrieved. Now more space-borne remote sensors are being used, such as optic devices, as well as real and synthetic aperture radars. We focus in determining advantages and limitations of each method to observe and retrieve directional properties of ocean surface waves. It seems that the various methods complement each other, while we critically exploit the data to determine the accuracy and resolution of wave directional information. Short wave directionality plays an important role in the final directional wave spectrum retrieved, specially under the influence of the observation geometry associated with the wind and wave relative directions.

How to cite: Ocampo-Torres, F. J., Osuna, P., Rascle, N. G., Herrera Vázquez, C. F., García-Nava, H., Díaz Méndez, G., Esquivel Trava, B., Villarreal-Olavarrieta, C. E., and Mora-Escalante, R. E.: Directional wave spectrum retrieved from in-situ and remote sensors, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13092, https://doi.org/10.5194/egusphere-egu25-13092, 2025.

EGU25-13185 | ECS | Orals | OS1.10

Assessing the Inter-annual variability of energy contained by wind waves in the tropical Indian Ocean 

Thanvi Rahman, Raveendran Sajeev, and Sheela Nair

The study investigates the inter-annual variability of energy contained by wind waves over the tropical Indian Ocean using Empirical Orthogonal Function (EOF) analysis. Emphasizing the first two leading modes of variability, the regions with significant changes in wind wave power over the last four decades are identified utilizing reanalysis data sets spanning between 1979 to 2023. In the first two EOF modes, accounting for 36.29% and 14.56% of the total variance respectively, the variability exhibited is highest in the Tropical Southern Indian Ocean region.

The leading mode of variability (EOF 1) exhibits multiple distinct lobes of high variability, including the southern tropical Indian Ocean region (10°S–30°S, 70°E–100°E), the southwest Arabian Sea, the southeastern tip of the Indian Ocean, and the southeastern equatorial Indian Ocean, which shows contrasting trends. Notably, these regions of high variability align precisely with the zones of extreme values in the annual climatology of energy flux input into surface waves over the tropical Indian Ocean computed for the same study period. Although wind speed is often used as a general proxy to explain and reason wave power variability, the parameter ‘energy flux input into surface waves’ demonstrates the closest and precise resemblance to zones of spatial variability of wave power in the study region, as it directly measures the energy transfer from wind to waves, accounting for critical factors such as air-sea coupling, wave age, and sea state. Considering this, the study also examines the met-ocean parameters that influence the energy flux input into surface waves. The climatology and long-term variability of parameters such as wind stress, wave steepness, and wave age in the study region were analysed. Additionally, the relative contribution of each parameter to wave power variability in the region was assessed.

In EOF Mode 2, the entire study region, excluding the Arabian Sea and the Bay of Bengal, exhibits a clear contrasting pattern between the eastern and western sides, with a prominent dipole pattern observed in the tropical southern Indian Ocean, spanning 10°S to 25°S and 55°E to 110°E.

This study offers insights into the long term variabilities in the energy contained by wind waves and to identify and analyze the met-ocean drivers influencing these variations and to assess their contribution.

Figure: Spatial Distribution of Inter-Annual variability in power of wind waves based on

(a) EOF1 and (b) EOF 2

                                            (a)

                                        (b)

How to cite: Rahman, T., Sajeev, R., and Nair, S.: Assessing the Inter-annual variability of energy contained by wind waves in the tropical Indian Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13185, https://doi.org/10.5194/egusphere-egu25-13185, 2025.

EGU25-14371 | Posters on site | OS1.10

Surface Gravity Wave Response to Air-Sea Coupling in the Gulf Stream Region: A Numerical Study 

Gwendal Marechal, Lionel Renault, Alexandre Barboni, Marco Larrañaga, and Bia Villas Bôas

In this study, a series of high-resolution coupled ocean-atmosphere-wave simulations are performed over the Gulf Stream to investigate the interactions between oceanic eddies and ocean surface waves. In particular, we investigate how ocean surface waves influence the dynamics of oceanic eddies and vice versa. To isolate the various feedback mechanisms, we perform dedicated simulations in which the contributions of each coupling - such as direct current-wave interactions, atmospheric feedbacks, and mesoscale oceanic features - are systematically removed from the air-sea wave coupling fields. Our results show, in agreement with observations, that oceanic eddies exert a significant influence on the surface waves, not only through direct current-wave interactions, but also by modulating the overlying atmospheric conditions. This modulation is manifested by the imprint of mesoscale oceanic features on the surface wind, which in turn affects the wave dynamics. Conversely, we also study the impact of ocean surface waves on the characteristics and statistics of oceanic eddies, providing insight into how wave-induced processes can modify eddy properties.

How to cite: Marechal, G., Renault, L., Barboni, A., Larrañaga, M., and Villas Bôas, B.: Surface Gravity Wave Response to Air-Sea Coupling in the Gulf Stream Region: A Numerical Study, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14371, https://doi.org/10.5194/egusphere-egu25-14371, 2025.

EGU25-15317 | ECS | Orals | OS1.10

Seasonal Wave Characteristics in the Presence of ENSO and IOD over the Bay of Bengal 

Subhashree Sahu, Hitesh Gupta, Rahul Deogharia, and Sourav Sil

Climatic modes like ENSO and IOD influence wind systems, which in turn can significantly impact the wave dynamics of a region. This study focuses on the changes in seasonal characteristics of waves induced by ENSO and IOD over the Bay of Bengal (BoB). We used monthly ERA-5 dataset of wind and wave parameters for 1980–2020. Based on Niño3.4 and dipole mode index, different phase of ENSO and IOD were selected. During the monsoon season, it was found that El Niño and La Niña increase significant wind wave height (Hsw) in the coastal regions, while they reduce the significant swell height (Hss) over the entire basin. However, the nIOD and pIOD enhance both the Hss and Hsw, albeit in different regions of the BoB. In post-monsoon season, when El Niño and La Niña are comparatively more active, they show similar features as pIOD and nIOD respectively. Reduced significant wave height (Hs), Hsw, and Hss in the entire BoB were noticed in the presence of El Niño and pIOD. However, these parameters were found to increase during La Niña and nIOD, especially in the eastern BoB. During winter, the signatures of the waves were much similar to those of post-monsoon but the magnitudes were comparatively low. During pre-monsoon of the next year, El Niño and pIOD showed signatures with increased Hss in the western BoB, whereas Hsw activity increased over the whole BoB. In presence of La-Niña and nIOD, a basin-wide increment in Hs, Hss, and Hsw is noticed. The aforementioned changes during different seasons were even more pronounced when El Niño & pIOD and La Niña & nIOD co-occurred. All these features noted in Hs, Hss, and Hsw during different seasons were found to co-vary with the spatial wind patterns, indicating winds to be a primary driver of these wave activities.

How to cite: Sahu, S., Gupta, H., Deogharia, R., and Sil, S.: Seasonal Wave Characteristics in the Presence of ENSO and IOD over the Bay of Bengal, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15317, https://doi.org/10.5194/egusphere-egu25-15317, 2025.

Few studies have focused on the projected future changes in wave climate in the Chinese marginal seas. In this study, we investigate the projected changes of the extreme wave climate over the Bohai Sea, Yellow Sea, and East China Sea (BYE) under the RCP2.6 and RCP8.5 scenarios from WAM wave model ensemble simulations with a resolution of 0.1 degree This is currently the highest-resolution wave projection dataset available for the study domain. The wind forcings for WAM are from high-resolution (0.22 degree) regional climate model (RCM) CCLM-MPIESM simulations. The multivariate bias-adjustment method based on the N-dimensional probability density function transform is used to correct the raw simulated significant wave height (SWH) and mean wave period (MWP). We investigated the projected changes in frequency, intensity and duration of extreme wave events under different warming levels. Uncertainty in projected changes of extreme wave has been analyzed and results show that model uncertainty is the dominant contribution to the total uncertainties of wave projections.

How to cite: Li, D., Liu, H., and Yin, B.: High-resolution Dynamical Projections and Uncertainty assessment of the Extreme Wave Climate for China's offshore under different global warming levels, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15849, https://doi.org/10.5194/egusphere-egu25-15849, 2025.

EGU25-16980 | Orals | OS1.10

Advancing High-Resolution Downscaling of Wind-Generated Ocean Waves Using WW3 on Unstructured Grids 

Aron Roland, Ali Abdolali, Tyler Hesser, Heloise Michaud, David Honegger, Mary Bryant, Thomas Huxhorn, and Jane M. Smith

Accurate modeling of wind-generated ocean waves is critical for understanding coastal processes, maritime operations, and coastal management. Recent advances in global wave forecasting have substantially improved large-scale predictions; however, bridging the gap between coarse-scale solutions and the finer-resolution requirements of nearshore environments remains an ongoing challenge. In this study, we present our latest developments in numerically downscaling wind-wave fields using the WAVEWATCH III (WW3) framework on unstructured grids, enabling more flexible resolution in complex coastal and shallow-water settings.

We detail a series of enhancements in WW3 aimed at improving both precision and computational efficiency. These include a new limiter implementation within the implicit scheme, GSE correction, and refined numerical integration of shallow water source terms and wave setup computations. In addition, we have optimized memory management and parallelization across the WW3 code base. By applying these techniques to a range of configurations, from simplified wind-wave growth scenarios to high-resolution global unstructured-grid models, we illustrate the upgraded performance and broad applicability of WW3, including its potential for more accurate wave climate assessments.

Lastly, we showcase a novel wave modeling framework based on a recent C++ language implementation of the unstructured solver. This approach leverages SIMD-based vectorization at the CPU level (0-level parallelism) in conjunction with domain decomposition and hybrid MPI+OpenMP parallelism, resulting in significant computational speed-ups. Such gains are especially valuable for long term runs of high resolution simulations, highlighting the framework’s suitability for future climate modeling efforts that demand high-resolution wave climatology over extended temporal scales.

How to cite: Roland, A., Abdolali, A., Hesser, T., Michaud, H., Honegger, D., Bryant, M., Huxhorn, T., and M. Smith, J.: Advancing High-Resolution Downscaling of Wind-Generated Ocean Waves Using WW3 on Unstructured Grids, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16980, https://doi.org/10.5194/egusphere-egu25-16980, 2025.

EGU25-18481 | Posters on site | OS1.10

Improving Global Wave Spectrum Representation Through SWH Assimilation and Spectral Reconstruction in WaveWatch III 

Hyeonmin Lee, Kyeong Ok Kim, Hanna Kim, Sang Myeong Oh, and Young Ho Kim

This study applies the Ensemble Optimal Interpolation (EnOI) method to assimilate significant wave height (SWH) data into the WaveWatch III global ocean wave model and evaluates the impact of wave spectrum reconstruction techniques on model performance. The results demonstrate significant reductions in root mean square errors (RMSE) for significant wave height predictions, particularly in most oceanic regions except for the equatorial zones. The assimilated fields enhanced the spectral representation of the WaveWatch III model, substantially improving the accuracy of global wave simulations. This study emphasizes the potential of EnOI-based SWH data assimilation and spectral reconstruction techniques in advancing ocean wave modeling and provides valuable insights for future ocean prediction and operational applications

How to cite: Lee, H., Kim, K. O., Kim, H., Oh, S. M., and Kim, Y. H.: Improving Global Wave Spectrum Representation Through SWH Assimilation and Spectral Reconstruction in WaveWatch III, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18481, https://doi.org/10.5194/egusphere-egu25-18481, 2025.

EGU25-21482 | Orals | OS1.10 | Highlight

On long term assessement of improved ocean/wave coupling in the Southern Ocean and Marginal Ice Zone 

Lotfi Aouf, Emma Bedossa, and Herve Giordani

The Southern Ocean is strongly affected by uncertainties on the surface wind, and consequently the fluxes exchanged between the atmosphere and the ocean include fairly strong biases. The assimilation of directional wave spectra from wave scatterometer SWIM of CFOSAT has demonstrated the improvement of the prediction of the different scales of waves from the wind-waves to the swell. As a result, the estimation of momentum and heat fluxes are positively affected, particularly in the western boundary current regions. This work presents long term validation of key ocean parameters (temperature, current and salinity) in the Southern Ocean from coupled experiments of the MFWAM and NEMO models over a long period of 4 years. Simulations with and without the assimilation of SWIM spectra are compared to estimate the impact on ocean circulation.


The ocean model outputs have been validated with the available level 3 & 4 in situ and satellite observations over the Southern Ocean. A comparison was made with climatologies for some parameters such as the ocean mixed layer. The results indicate a significant impact on the heat content at 300 m depth in the Southern Ocean, particularly in the marginal ice zone. The analysis of temperature and salinity profiles over specific locations in the MIZ shows good consistency of variability with the coupled simulation using CFOSAT assimilation. In this work we investigated the impact of using wave/ice interaction in the coupling. We also examined the use of Eddy diffusivity Mass fluxes (EDMF) convection scheme in NEMO model and evaluate the impact on ocean circulation in the southern ocean. Further comments and conclusions will be reported in the final presentation.

How to cite: Aouf, L., Bedossa, E., and Giordani, H.: On long term assessement of improved ocean/wave coupling in the Southern Ocean and Marginal Ice Zone, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21482, https://doi.org/10.5194/egusphere-egu25-21482, 2025.

NP8 – Emergent Phenomena in the Geosciences

EGU25-848 | ECS | Posters on site | CL3.2.4

Heat Stress Threats in Europe: A Comprehensive Analysis of sWBGTVariations and Trends (1979 -2023) 

Qi Zhang, Joakim Kjellsson, Emily Black, and Julian Krüger

Heat stress has lately been acknowledged as a significant threat to public health, with heat waves becoming more frequent and severe due to global warming. The Simplified Wet Bulb Globe Temperature (sWBGT) is a effective indicator for heat stress, combining both temperature and relative humidity. Using observations and reanalysis datasets, we identify annual heatwave days (HWD) and analyze sWBGT variations and trends during HWD. We focus on three European regions: Northern Europe (NEU), Western and Central Europe (WCE), and the Mediterranean (MED). We observed an increasing trend in sWBGT over most of Europe , with the exception of areas around the Black Sea, parts of eastern and western WCE, and the western MED. Importantly, the  contribution of temperature and humidity on heat stress vary by regions. In NEU, positive trends in both temperature and relative humidity contribute to increased heat stress, with temperature showing a more significant rising trend (0.4°C/decade). In WCE, while the overall trend in sWBGT is positive, changes in relative humidity are minimal (0.007% /decade), with temperature trends being the primary driver. In MED, a positive trend in sWBGT of 0.3 /decade is a residual of a  negative trend in relative humidity and a positive temperature trend. Comparing ERA5 dataset with meteorological station data revealed biases in the ERA5 data in Mediterranean cities with pronounced urban heat island effects. Analysis of sWBGT threat levels showed that NEU and WCE regions currently remain at safe levels. In contrast, most MED regions are at alert levels, with some areas escalating to caution levels. Our research provides comprehensive insights into heat stress variations across European regions over recent decades. This work can provide scientific evidence to help policymakers develop effective adaptation to address potential future heat stress threats.

How to cite: Zhang, Q., Kjellsson, J., Black, E., and Krüger, J.: Heat Stress Threats in Europe: A Comprehensive Analysis of sWBGTVariations and Trends (1979 -2023), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-848, https://doi.org/10.5194/egusphere-egu25-848, 2025.

EGU25-916 | ECS | Orals | CL3.2.4

Atmospheric and Oceanic Processes Behind Extreme Precipitation: A Case Study of the Western Ghats 

Leena Khadke, Sachin Budakoti, Akash Verma, Moumita Bhowmik, and Anupam Hazra

India has experienced a notable rise in the intensity, frequency, and spatial extent of extreme weather events in recent decades, with extreme precipitation along the southwest coast being particularly alarming. The drivers behind these events remain uncertain due to the variability in meteorological and oceanic factors and associated large-scale circulations. The present study attempted to identify a combination of dynamic, thermodynamic, and cloud microphysics processes contributing to the anomalous precipitation over the southwest coast of India from 1-10 August 2019 against its climatology using reanalysis and observational datasets. Key findings reveal the critical role of warm sea surface temperature anomalies (>1.4°C), reduced outgoing longwave radiation (<-50 W/m²), and elevated atmospheric temperatures (>1.6°C over the ocean) in enhancing atmospheric moisture capacity by nearly 10%. Strengthened low-level winds (anomalies >4 m/s) transported this moisture from the ocean to the land, while vertical updrafts (> -0.4 m/s anomalies) increased atmospheric instability and moisture convergence. Additionally, significant anomalies in cloud hydrometeors (>2.5×10⁻⁴ Kg/Kg) supported prolonged intense precipitation. These results improve our understanding of the interaction between ocean-atmosphere dynamics and wind patterns, highlighting their vital role in shaping regional weather and climate.

Keywords: Extreme precipitation, Western ghats, Atmospheric processes, Reanalysis.

How to cite: Khadke, L., Budakoti, S., Verma, A., Bhowmik, M., and Hazra, A.: Atmospheric and Oceanic Processes Behind Extreme Precipitation: A Case Study of the Western Ghats, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-916, https://doi.org/10.5194/egusphere-egu25-916, 2025.

EGU25-1049 | ECS | Posters on site | CL3.2.4

Analysis of projected monthly changes of extreme temperature indices to support decision-makers 

Ferenc Divinszki, Anna Kis, and Rita Pongrácz

As global warming intensifies, the building of adaptation and mitigation strategies has become an urgent task. In the centre of these strategies often lie extreme weather events, which are expected to become even more severe and more frequent in the next decades. Therefore, extending our knowledge on the potential changes in these events is crucial to provide assistance for appropriate preparation and planning necessary actions. Using the latest CMIP6 global climate model simulations available in the IPCC’s Interactive Atlas (IA), a study on extreme events focusing on Europe was completed, with special emphasis on Central Europe.

Our goal was to study the potential changes of extreme temperatures over the continent, in order to analyse the spatial patterns and trends of changes for the end of the 21st century. First, monthly multi-model mean data were downloaded from the IA for two different extreme temperature indices. The number of days with maximum temperature above 35 °C (i.e. TX35) and the number of days with a minimum temperature below 0 °C (i.e. frost days or FD) were selected for the analysis. The use of both hot and cold extreme temperature indices enabled us to cover every month in our study with TX35 analysed in the May–September and FD in the October–April period. Our target period was the 2081–2100 period compared to the values of 1995–2014 (i.e. the last two decades of the historical simulation period) as a reference. Every scenario available in the IA was considered, namely, SSP1-2.6, SSP2-4.5, SSP3-7.0 and SSP5-8.5.

Six zonal segments were defined over Europe to analyse the projected changes, ensuring that the segments fairly cover the continent. This approach is able to reveal the major effects creating the spatial patterns in different regions. The most important effects are (i) the differences due to the north-south or east-west locations (i.e. the zonal and continental effects), (ii) elevation above sea level (i.e. the orographical effect), and (iii) the different levels of anthropogenic forcing (i.e. the different scenarios).

Our results show that the anthropogenic effect is a key factor due to the direct connection between the greenhouse effect and air temperature. Moreover, the sea-land surface differences have the greatest effect on the magnitude of changes in the indices, while continentality is also an important factor. Potential differences due to elevation, however, are often supressed by the spatial patterns created by sea-land differences.

How to cite: Divinszki, F., Kis, A., and Pongrácz, R.: Analysis of projected monthly changes of extreme temperature indices to support decision-makers, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1049, https://doi.org/10.5194/egusphere-egu25-1049, 2025.

EGU25-1556 | ECS | Orals | CL3.2.4

A global Lagrangian analysis of near-surcface warm and cold temperature extremes 

Amelie Mayer and Volkmar Wirth

Temperature extremes have a substantial impact on society and the environment, however a full physical understanding of their formation mechanisms is still lacking. In particular, the relative importance of the three key processes – horizontal temperature transport, subsidence accompanied by adiabatic warming, and diabatic heating – is still debated. Here, we present a global quantification of the contributions from these processes to near-surface warm and cold extremes using the Lagrangian framework. To this end, we apply two different Lagrangian temperature anomaly decompositions: one based on the full fields of the respective terms, and the other one based on the anomaly fields of the respective terms (i.e., deviations from their corresponding climatologies). We will show that the results from the full-field decomposition mostly align with those of a previous study, while the anomaly-based decomposition offers a completely new assessment of the roles of the different processes, especially with regard to warm extremes.

How to cite: Mayer, A. and Wirth, V.: A global Lagrangian analysis of near-surcface warm and cold temperature extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1556, https://doi.org/10.5194/egusphere-egu25-1556, 2025.

EGU25-1678 | Orals | CL3.2.4

How do transitions from dry to wet states propagate to drought-to-flood transitions? 

Manuela Irene Brunner, Bailey Anderson, and Eduardo Munoz-Castro

Transitions from dry to wet states challenge water management and can lead to severe impacts on infrastructure and water quality. Such transitions occur both in the atmosphere and hydrosphere, that is, from dry-to-wet spells and from droughts to floods, respectively. While transitions from dry-to-wet spells, i.e. from negative to positive precipitation anomalies, are relatively well studied, it is yet unclear how they propagate to hydrological transitions from negative to positive streamflow anomalies. Here, we address the question of how often, where, when, and why meteorological transitions do propagate to drought-to-flood transitions using a large-sample dataset of precipitation and streamflow observations over Europe. Our analysis of the relationship between meteorological and hydrological transition events shows that only 10% and 25% of the dry-to-wet transitions propagate to drought-to-flood transitions at a monthly and annual time scale, respectively. The limiting factors for transition propagation are clear differences in the seasonality of meteorological and hydrological transitions and the limited propagation of wet spells, in particular those with low precipitation intensities and small volumes. Transition propagation is most likely in small and rainy catchments, that is, catchments with a relatively direct link between precipitation and streamflow and limited storage influences. We conclude that hydrological transitions are only weakly related to meteorological transitions, which highlights the important influence of land-surface and storage processes for the development of hydrological transitions. As a consequence, changes in dry-to-wet transitions are a relatively poor proxy for future changes in drought-to-flood transitions.

How to cite: Brunner, M. I., Anderson, B., and Munoz-Castro, E.: How do transitions from dry to wet states propagate to drought-to-flood transitions?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1678, https://doi.org/10.5194/egusphere-egu25-1678, 2025.

Humid heatwaves negatively affect human health due to the integrating effect of temperature and humidity, and thus the early warning and timely mitigating on climate extremes are essential. Yet, systematic assessment on the intra‐annual onset and end of humid heatwaves, which is associated to the occurrence of first and last humid heatwaves, are missing globally. Using a new station‐based data set of daily maximum wet‐bulb temperature, the start and end dates, cumulative anomaly and extremely humid heat of the first and last humid heatwaves in the Northern Hemisphere were explored. It was found that at 91.54% of stations, humid heatwaves started earlier or ended later in the period of 2001–2020 compared to 1981–2000. High cumulative anomalies of the first or last humid heatwaves were found in the mid‐ and high‐latitude regions. Average difference between all humid heatwaves and the first humid heatwaves in cumulative anomalies increased steadily at stations north of 35°N. At regional scales, South East Asia had become the most prominent area with intensification of intra‐annual onset and end of humid heatwaves and will experience more frequent extreme events by 2100.

Furthermore, our focus goes from physical understanding to exposure impacts. Human exposure to humid heatwaves develops with the significant intensification of extreme humid-heat and population agglomeration. Although urban areas are typical spaces of the heat stress, urban heat is expanding outward to rural areas spatially. However, the difference of long-term changes and attributions between urban and rural human exposure to humid heatwaves is still unclear, especially lacking global comparisons supported by continuous series. We also used the new wet-bulb temperature dataset and integrated scenario data to assess historical and future human exposure to humid heatwaves in the Northern Hemisphere. The differences between urban and rural areas in the contribution of enhanced heatwaves and increasing population were quantified. The results showed that about 96.62 % of the stations had pronounced increases in human exposure among those with significant changes. The domination of enhanced heatwaves to human exposure rate was stronger in urban areas in typical developed countries, while domination of increasing population was higher in rural areas in eastern China, with 87.5 % of rural stations dominated by population growth. Under extremely increasing conditions in SSP5 scenario, average rates of human exposure to humid heatwaves in rural areas would be 11.78 % higher than urban areas.

Our findings demonstrated more intensified characteristics of the intra‐annual onset and end of humid heatwaves and provide a scientific cognition for the local risk of humid heatwaves.

How to cite: Dong, J.: Intra‐annual occurrence and risk of humid heatwave in the Northern Hemisphere, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2790, https://doi.org/10.5194/egusphere-egu25-2790, 2025.

EGU25-2889 | ECS | Orals | CL3.2.4

Storyline climate attribution for compound flooding from tropical cyclone Idai in Mozambique.  

Doris Vertegaal, Bart van den hurk, Anaïs Couasnon, Natalia Aleksandrova, Tycho Bovenschen, Simon Treu, Matthias Mengel, and Sanne Muis

It is widely recognized that climate change is altering the likelihood and intensity of extreme weather events globally, including hydrological extremes such as floods. Compound flooding is driven by fluvial, pluvial and coastal flooding occurring simultaneously, resulting in a potentially larger impact when co-occurring than the sum of the univariate drivers happening separately. Identifying and communicating the effect of climate change on compound flooding remains challenging. A method to quantify the effect of climate change on these events is through climate attribution assessments. 

This research assesses how existing climate attribution methods can be applied to compound events instead of univariate events. An event-based storyline attribution approach for compound flooding from historical tropical cyclones (TCs) in Mozambique is used to examine the effect of climate change on multiple flood drivers propagated to impact. TC Idai hit Mozambique in 2019 and caused over 600 fatalities, affected over 1.8 million people, resulting in $3 billion in damages. Idai is used as a case study, representing a highly destructive compound flood event. 

Compound flooding is modelled using a state-of-the-art hydrodynamic modelling chain that combines the Super-Fast INundation for coastS (SFINCS) model with the hydrodynamic model Delft3D Flexible Mesh and hydrological model wflow, linked to a fast impact assessment tool Delft-FIAT to calculate the flood impact, here the direct economic damages. The drivers of compound flooding from TCs that are known to be affected by climate change, such as precipitation, wind and sea-level rise, are adjusted to create counterfactual scenarios. The compound flooding is modelled for the multiple factual and counterfactual scenarios, adjusting the separate drivers individually and simultaneously.  

This approach enables the attribution of climate change effects on compound flooding from TCs while identifying potential changes in the contributions of individual flood drivers. Next steps include attribution uncertainty partitioning, comparing multiple climate attribution approaches for these events, assessing regional differences with relation to climate change effects on compound flood impact and comparing this methodology for multiple TCs in the same region, which may have different driver contributions.

How to cite: Vertegaal, D., van den hurk, B., Couasnon, A., Aleksandrova, N., Bovenschen, T., Treu, S., Mengel, M., and Muis, S.: Storyline climate attribution for compound flooding from tropical cyclone Idai in Mozambique. , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2889, https://doi.org/10.5194/egusphere-egu25-2889, 2025.

EGU25-3474 | ECS | Orals | CL3.2.4

Dynamical evolution of extremely hot summers in Western Europe in response to climate change 

Robin Noyelle, Arnaud Caubel, Yann Meurdesoif, Davide Faranda, and Pascal Yiou

The study of the statistical and dynamical characteristics of extreme and very extreme events in the climate system is impaired by a strong under-sampling issue. Here we use a rare events algorithm to massively increase the number of extremely hot summers simulated in the state-of-the-art IPSL-CM6A-LR climate model under present and future anthropogenic forcings. This allows us to reach precise climatological results on the dynamics leading to centennial hot summers. We demonstrate that the dynamics leading to these hot summers tend to be more local and less large scale-organized with climate change. In the future, high temperatures are still reached via a large anticyclone, but anomalies do not extend as far longitudinally as in the present and arise mainly as a result of an increase in the intensity of surface heat fluxes.

How to cite: Noyelle, R., Caubel, A., Meurdesoif, Y., Faranda, D., and Yiou, P.: Dynamical evolution of extremely hot summers in Western Europe in response to climate change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3474, https://doi.org/10.5194/egusphere-egu25-3474, 2025.

EGU25-4554 | ECS | Orals | CL3.2.4

Future Changes to Extreme Rainfall over Puerto Rico in an Ensemble of Convection-Permitting Simulations 

Erin Dougherty, Andreas Prein, and Paul O'Gorman

Puerto Rico is a tropical island that frequently receives heavy rainfall from a variety of systems, including tropical cyclones like Hurricane Maria (2017), mesoscale convective systems (MCSs), and isolated convection. Its two distinct rainy seasons are dictated by moisture convergence associated with the North Atlantic Subtropical High, while sea breezes and complex topography influence precipitation on the mesoscale. Previous research has examined how tropical precipitation could change in a future climate, showing a decrease in precipitation by 2100 using global climate models (GCMs). However, relatively little research has been conducted using convection-permitting climate models over the tropical Atlantic to understand how precipitation extremes could change in a warmer climate. Here, we fill this gap by dynamically downscaling a 0.25 degree GCM 10-member ensemble to 3 km using the Model Prediction Across Scales (MPAS) model for extreme precipitation events in a current (2001-2021) and future climate (2041-2061) over Puerto Rico. We show that MPAS is largely able to reproduce extreme precipitation events in the current climate when compared to observations and captures a variety of systems. We explore how future changes in extreme rainfall events in the early rainy season, which are largely driven by MCSs and isolated convection, compare to changes in the late rainy season, which are primarily due to tropical cyclones. 

How to cite: Dougherty, E., Prein, A., and O'Gorman, P.: Future Changes to Extreme Rainfall over Puerto Rico in an Ensemble of Convection-Permitting Simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4554, https://doi.org/10.5194/egusphere-egu25-4554, 2025.

Possibility of the occurrence of extreme weather and climate is often predicted in recent climate impact studies under certain global warming scenarios using climate models. However, it is usually unclear how such weather extremities occur as the resolution of the current generation climate models is not good enough to resolve individual storm system let alone pinning down the physical mechanisms. This ambiguity in physical mechanism impedes the better understanding of the nature of these extreme weather/climate events and can lead to ineffective mitigation and/or adaptation measures. For example, when the term extreme rainfall is mentioned, it is unclear whether it is caused by severe convective storms or by regular storms that have higher liquid water contents (LWC), as both can lead to large amount of rainfall. But the detailed physical mechanisms of these two types of storms are different. Clearly it is desirable to remove such ambiguity and clarify what type of storms would occur in certain climate regime.

 In this study, we utilize the meteorological series derived from the REACHES climate database compiled from Chinese historical documents (Wang et al., 2018; 2024) as well modern weather data to pin down the type of storms and the respective physical mechanisms responsible for the extreme events that preferably occur in cold versus warm climate regime. We use the REACHES reconstructed temperature series in China in 1368-1911 and construct convection index series to show that the severe deep convective storms are the preferable type that causes extreme weather events in cold climate regime and utilize modern observational data to demonstrate that the high LWC (but not necessarily severe) storms are the type most likely to lead to extreme events.

Finally, physics-based storm model simulation results will be used to illustrate the dynamical processes of these two types of storms and explain why they lead to different precipitation patterns.  

How to cite: Wang, P. K.: Extreme weather types and their physical mechanisms in cold versus warm climate regimes: evidence from historical and modern climate data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4671, https://doi.org/10.5194/egusphere-egu25-4671, 2025.

EGU25-5022 | Orals | CL3.2.4

Human and land exposure to future recurrent unprecedented extremes 

Jonathan Spinoni, Marta Mastropietro, Carlos Rodriguez-Pardo, and Massimo Tavoni

In the last decades, highly impacting climate extremes have become increasingly frequent in many different global hotspots. According to climate projections, such events are likely to become even more severe during the 21st century, to the point that under the less conservative scocio-economic scenarios, they could become so recurrent that they possibly constrain the ability to adapt and mitigate, especially in poorly developed countries.


This study investigates the future occurrence of unprecedented heatwaves, droughts, rainfall and snowfall, namely the time of their emergence and when and where they will become the new climate normals, defined here as at least one such event any other year. As input data, we use an ensemble of high-resolution bias-adjusted climate simulations from the ISIMIP3b family and we focus on four SSPs (SSP1 to SSP5, excluding SSP4). Using population, land-use, and GDP projections without climate change, we also analyse their exposure to such unprecedented climate extremes from 2041 to 2100, focusing on continental and macro-regional scales.


We also present preliminary results obtained by using emulated scenarios, with a special focus on the possibility of preventing such unprecedented extremes under low-emission scenarios (SSP1-1.9 and SSP1-2.6) with specific temperature overshoot trajectories. We show that limiting frequent record-breaking heatwaves and droughts could be highly beneficial, especially in regions with lower income and higher vulnerabilities as Africa and Latin America.


The results presented in this study are included in the framework of the EUNICE project, which aims at quantifying the economic and non-economic impacts of future climate extremes, providing robust quantification of uncertainties. 

How to cite: Spinoni, J., Mastropietro, M., Rodriguez-Pardo, C., and Tavoni, M.: Human and land exposure to future recurrent unprecedented extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5022, https://doi.org/10.5194/egusphere-egu25-5022, 2025.

EGU25-5625 | ECS | Orals | CL3.2.4

The importance of internal variability for climate extreme indices 

Leonard Borchert, Benjamin Poschlod, Lukas Brunner, Vidur Mithal, Natalia Castillo, and Jana Sillmann

The occurrence of climate extremes is influenced by climate forcing as well as internal climate variability: internal variability may temporarily obscure or enhance the forced signal in climate extremes. The role of signal versus noise plays an important role, for instance in the analysis of emergence. The climate extreme indices from the Expert Team on Climate Change Detection and Indices (ETCCDI) are routinely used to assess the impacts of forced change on climate extremes, but in such analyses internal variability is often ignored. We present a comprehensive catalogue of the importance of internal variability for the 27 ETCCDI indices to inform climate extreme analysis and guide impact science.

In our assessment, we use a 50-member ensemble of the CMIP6 generation MPI-ESM 1.2 LR Earth System Model for 1961-2014 to highlight combinations of regions and indices that are strongly affected by internal variability. Unlike previous work, we consider all ETCCDI indices in the same model ensemble to provide a clean identification of internal variability. Using the coefficient of variation as initial metric, we find that the total signal is strongly affected by internal variability  

  • over ocean regions for temperature indices based on percentile thresholds (e.g. tx90p), 
  • along quasi-zonal mid-latitude bands for absolute maximum/minimum temperature indices (e.g. txx), and 
  • in characteristic (sub-)tropical “hot-spot” regions such as northern Africa, the eastern central Pacific, and the south-east of all ocean basins for precipitation-based indices (e.g. r95p). 

This grouping illustrates the differing relative importance of internal variability for the extreme signal depending on the index and the region, and sheds light on processes that contribute to the occurrence of climate extremes. Further, the catalogue provides a tangible resource that enables users of ETCCDI indices to better understand the robustness of index information they might derive from single model runs or observations. Based on our catalogue, users, e.g. impact scientists, may select suitable indices specific to their region of interest and application.

How to cite: Borchert, L., Poschlod, B., Brunner, L., Mithal, V., Castillo, N., and Sillmann, J.: The importance of internal variability for climate extreme indices, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5625, https://doi.org/10.5194/egusphere-egu25-5625, 2025.

EGU25-6589 | Orals | CL3.2.4 | Highlight

The perfect storm: loss potential of Eunice-like cyclones in a counterfactual climate 

Nicholas Leach, Shirin Ermis, Aidan Brocklehurst, Dhirendra Kumar, Alexandros Georgiadis, Lukas Braun, and Len Shaffrey
Storm Eunice was a severe windstorm that impacted Central Europe in February 2022, causing over €2.5 Bn in insured loss. It formed on a cold front west of the Azores before undergoing explosive cyclogenesis and tracking across Central Europe, producing recorded wind gusts of up to 55 ms-1. The contribution of climate change to the storm dynamics and severity was examined by Ermis et al., who found that in counterfactual weather forecasts - given an identical initial synoptic setup - climate change had measurably increased the severity of the storm. 
 
Here we move beyond their meteorological attribution and quantify the role of climate change in the losses incurred during Eunice. We combine the same counterfactual weather forecasts with two loss models, including one state-of-the-art catastrophe model, finding that the increases in meteorological severity do translate through to substantial increases in estimated loss. We compare the loss model results with a commonly used “loss index” finding that the index inadequately represents the heavy tail of the loss distribution, demonstrating the importance of using impact models for quantitative assessments of loss in a changing climate.
 
Of particular note is the existence of several “boosted” members within the forecast ensembles whose losses are far greater than what unfolded in reality. This includes one realisation, simulated in a warmer “future” climate, in which the total loss nearly reaches €50 Bn. The plausible existence of such a catastrophic loss is of considerable relevance to a wide variety of stakeholders across adaptation planning, and the financial sector. We suggest that our results demonstrate not only the potential utility of weather forecast models in quantifying impacts attributable to climate change, but also the value of academic - private partnerships in which the two sectors are able to bring different areas of expertise.

How to cite: Leach, N., Ermis, S., Brocklehurst, A., Kumar, D., Georgiadis, A., Braun, L., and Shaffrey, L.: The perfect storm: loss potential of Eunice-like cyclones in a counterfactual climate, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6589, https://doi.org/10.5194/egusphere-egu25-6589, 2025.

EGU25-6594 | ECS | Posters on site | CL3.2.4

A Counterfactual Emulator for Circulation-Driven Extremes in Southeast Asia 

Xinyue Liu, Xiao Peng, and Xiaogang He

Climate extremes jeopardize human health and the environment. Recent unprecedented extremes suggest a complex interplay between anthropogenic warming and internal variability of the climate system, with large-scale circulations exhibiting considerable uncertainty in response to climate change. Therefore, understanding the influence of large-scale atmospheric and oceanic circulations on extreme events in a changing climate is crucial for climate adaptation and risk assessment. Traditional physical climate models, while powerful, require extensive computational resources to explore the broad spectrum of potential future circulation states and their implications for the infrequent occurrence of extreme events. This study takes Southeast Asia as an example to demonstrate the influence of Madden–Julian Oscillation (MJO) on extreme precipitation and droughts in a changing climate, as MJO strongly modulates local convective systems in Southeast Asia. We develop an AI-empowered emulator framework based on a conditional diffusion model to generate the precipitation field in a counterfactual world, where the enhanced convective phases of MJO are more (less) frequent than the current climate. We then estimate the intensity-frequency curves of extreme precipitation (drought) events and quantify the uncertainty using the generated large ensemble of samples. This counterfactual emulator allows us to isolate the influence of MJO phases and frequencies on extreme event probabilities, making it feasible to simulate a wide array of circulation states and examine their impacts under various climate change scenarios. By overcoming computational barriers, the study offers a clearer understanding of climate extremes in response to changing circulations for policymakers and stakeholders, enabling climate-informed resilience planning and evidence-based governance policy.

How to cite: Liu, X., Peng, X., and He, X.: A Counterfactual Emulator for Circulation-Driven Extremes in Southeast Asia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6594, https://doi.org/10.5194/egusphere-egu25-6594, 2025.

Between July 19 and 24, 2023, a multi-day outbreak of severe convective storms impacted Europe, affecting several countries. Northern Italy experienced multiple severe storms during this period, with July 24 marking the most intense day, particularly for hailstorms. On this day, three long-lived hailstorms caused significant damage, injured 119 people, and produced the largest hailstone ever observed in Europe—and the second largest globally—with a diameter of 19 cm. Recent studies highlight positive trends in both the frequency and intensity of convective environments favorable to thunderstorm activity in this region, alongside an increase in reports of large hail events.

This case study examines these trends in the context of the July 24, 2023, event, aiming to determine whether significant changes have occurred that may have increased the likelihood or severity of such an event. We employ a storyline approach based on circulation analogs to analyze the atmospheric conditions leading to this hailstorm.

Results show that similar events are fuelled by much larger CAPE today compared to just a few decades ago, likely linked to the strong upward trend in Mediterranean sea surface temperatures, coupled with a modest decrease in bulk wind shear. Additionally, the data suggest a potential intensification of the dynamics underlying similar configurations over the past 70 years, due to steepening of the horizontal geopotential gradient across the region. 

How to cite: Pons, F.: Analogs-based attribution of the July 24th, 2023 extreme hail storms in northeastern Italy, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6770, https://doi.org/10.5194/egusphere-egu25-6770, 2025.

Extreme weather events have been increasing as global temperatures rise. Semi-enclosed basins such as the Black Sea and the Mediterranean are particularly susceptible to extreme weather due to their unique topographic features and land-sea distribution. Extreme precipitation events on the north-facing slopes of the mountains in the Black Sea Region occur due to relatively cold air interacting with the warm sea and being orographically lifted over the mountains. On August 10-12 2021, a deadly flash flood occurred on the coast of the Black Sea in Northern Türkiye which resulted in excessive precipitation (200-450 mm) causing loss of lives of 97 people and leaving 228 injured. We investigated extreme weather event which occurred near the Black Sea along with future climate conditions using the Pseudo-Global Warming method. In order to analyze the event, we used a numerical weather prediction model (WRF) in convection-permitting 3 km horizontal resolution with a domain covering the Black Sea and surrounding area. The model simulations are driven by ECMWF Reanalysis 5th Generation (ERA5) data for initial and boundary conditions. To derive climate change signals, we used 25 CMIP6 Earth System Models and eliminating the rest of the models that have no ocean model component over the Black Sea. The signals are computed for three different future periods (2025–2049, 2050–2074, and 2075–2099) relative to the 1990–2014 historical period. Each climate change signal which represents different periods were added to ERA5 6-hourly data as ensemble means. In the first future period (2025-2049), sea surface temperature (SST) in August is projected to increase by 1.7 °C, and by the end of the period (2075-2099), SST is expected to rise by 5 °C over the Black Sea. Additionally, while near-surface air temperatures in August are projected to increase by 1.5 °C to 2.5 °C initially, they are expected to rise by approximately 5.5 °C to 8.5 °C in the final period over the simulation domain. Moreover, near-surface relative humidity over land in August is simulated to decrease by nearly 10% in the last quarter of the century. The findings of this study will contribute to our understanding of how extreme precipitation events develop under future climate conditions and provide insights of the physical and dynamic processes that could drive these events in a warmer world.

How to cite: Şahinoğlu, S. and Önol, B.: Convective Permitting Simulations for Excessive Precipitation Event Under Pseudo-Global Warming in the Black Sea Region, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6834, https://doi.org/10.5194/egusphere-egu25-6834, 2025.

EGU25-8204 | Orals | CL3.2.4 | Highlight

Was July 2021 extreme rainfall in western Germany close to the worst possible?  

Vikki Thompson, Rikke Stoffels, Hylke de Vries, and Geert Lenderink

In July 2021 extreme rainfall associated with a cut-off low pressure system led to huge impacts in western Germany, Belgium, and the Netherlands. The event was costly both in terms of loss of life and insurance damages. We use a multi-method approach to examine the event and to assess whether it could have been even worse. Using atmospheric analogues from reanalysis, pseudo global warming simulations, and a boosted ensemble of a dynamically similar event we show that the observed rainfall pattern is highly sensitive to the large-scale dynamics. For example, although good dynamical analogues are found in reanalysis, these do not all show the same hazards – with many showing very little rainfall.  

Our results suggest the magnitude of rainfall experienced was very unusual, perhaps close to the worst possible in the current climate, as small dynamical changes lead to a drastic reduction of the rainfall. 

How to cite: Thompson, V., Stoffels, R., de Vries, H., and Lenderink, G.: Was July 2021 extreme rainfall in western Germany close to the worst possible? , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8204, https://doi.org/10.5194/egusphere-egu25-8204, 2025.

EGU25-8539 | ECS | Posters on site | CL3.2.4

Meteorological Conditions during Compound Wind and Precipitation Extremes in Coastal Southeast Asia 

Diah valentina lestari, Wei jian, and Edmond yatman lo

Compound precipitation and wind (CWP) extreme events can bring a destructive impact to cities located along coastal areas. Total seasonal occurrence of CWP extreme events reaches its highest number of more than sixty events per year in several coastal cities of Southeast Asia (SEA) with a peak occurrence during summer (June-September). This study investigates nine meteorological variables to identify linkages between atmospheric conditions and CWP extreme events using the Coordinated Regional Climate Downscaling Experiment for Southeast Asia (CORDEX-SEA) dataset. These nine variables are chosen due to their importance as trigger factors to convections and wind gusts, e.g. equivalent potential temperature to represent moist enthalpy and atmospheric static stability as affecting wind gusts. Twelve coastal cities across Vietnam (five cities), the Philippines (three cities), Thailand (two cities), Cambodia (one city), and Myanmar (one city) are grouped into four groups with similar climatological patterns of the nine meteorological variables during the historical summer period (1975-2005). All groups imply the importance of their regional underlying zonal and meridional wind anomaly, outgoing longwave radiation (OLR) anomaly, and low-level moisture flux conditions during CWP extreme events days. CWP days for Group 1 (Cebu, Davao, and Metro Manila) are associated with low-level moisture convergence, negative OLR anomaly, and stronger zonal wind anomaly that enhances the precipitation intensity and wind gusts. The presence of a low-pressure system over the northern part of Metro Manila may also influences the CWP extremes for Group 1. Similarly, as a group that is prone to tropical cyclones, Group 2 (Da Nang, Hanoi, and Hai Phong) are also affected by similar dominant factors as Group 1 with an additional factor from the meridional wind anomaly. Located in between the South China Sea and the Indian Ocean, Group 3 (Yangon, Bangkok, and Chon Buri) is dominantly affected by low-level moisture convergence, zonal wind anomaly, and warm-moist transports from the Indian Ocean. Group 4 (Can Tho, Ho Chi Minh City, and Phnom Penh) shows a similar metrological pattern as Group 3 without notable changes in warm-moist transports. The regional means of these nine meteorological variables are further applied to train a Support Vector Machine (SVM) with an additional unbalanced data handling stage prior to the model training process. The best-trained SVM model results in the highest f1 score of 0.78 and 0.76 on the model’s testing set for Group 3 and 4. Further evaluation of the trained SVM model shows that the model’s predictions on a testing dataset fall within the 95% confidence interval. The best model is next used to predict the occurrence of CWP extreme events in the summer of 2006-2023. This model results in a predictive f1 score of 0.61 for Group 3 and 0.54 for Group 4, corresponding to a total of 98% and 97% correctly predicted (true positive), respectively.

How to cite: lestari, D. V., jian, W., and lo, E. Y.: Meteorological Conditions during Compound Wind and Precipitation Extremes in Coastal Southeast Asia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8539, https://doi.org/10.5194/egusphere-egu25-8539, 2025.

EGU25-8602 | ECS | Orals | CL3.2.4

Climate change caused the catastrophic severity of Cyclone Daniel over Libya in 2023 

Laurenz Roither, Douglas Maraun, and Heimo Truhetz

Cyclone Daniel was the deadliest Mediterranean storm on record and struck Greece and Libya in September 2023. In our study, we aim to disentangle the factors contributing to the severity of the event, with a focus on the influence of anthropogenic climate change. To this end we utilized a process-based, conditional attribution approach and simulated storylines of the event with a convection permitting regional climate model under actual and counterfactual conditions. Specifically, we tested how cyclone Daniel would have unfolded (1) in a 1970s world with 1°C less climate change; (2) without the prevalent Mediterranean sea surface temperature anomaly of +1.3 °C; and (3) with decreased soil moisture in the Balkans assuming no rainfall anomalies had occurred in the months prior to the event. Climate response uncertainties have been approximately accounted for by imposing climate change signals from different GCMs. 

Our simulations show that 1°C of climate change only moderately influenced the cyclone's extreme precipitation during its early phase in Greece. In contrast, during its tropical-like Libyan phase, this level of climate change has amplified the severity of the event by a staggering 30 to 60%. Increased energy availability and convection led to the formation of a rare and destructive Medicane with a warm and rapidly deepening core. Artificially lowering only the sea surface temperatures reduced the meteorological hazards in both phases and underpins the importance of the Mediterranean as an energy and moisture source. Reducing soil moisture over the Balkans alone, although an important source for evapotranspiration during the early phase, did not substantially affect the intensity of the cyclone.

Our results demonstrate that current climate change can already be a game changer for individual extreme events and highlight the power of storylines to analyze the potentially destructive influence of climate change on rare extreme weather events.

How to cite: Roither, L., Maraun, D., and Truhetz, H.: Climate change caused the catastrophic severity of Cyclone Daniel over Libya in 2023, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-8602, https://doi.org/10.5194/egusphere-egu25-8602, 2025.

EGU25-9252 | ECS | Posters on site | CL3.2.4

How can the catastrophic risk potential of unseen climate extremes be understood? 

Tom Wood, Hebe Nicholson, Jenix Justine, and Tom Matthews

The Earth’s climate is heading into unprecedented territory, with the global mean surface temperature reaching record-breaking levels in 2024. Meanwhile, on regional scales, extreme events are becoming both more frequent and more severe, with some events being without precedent in the observational record. These types of ‘unseen’ events could result in very high-impact, potentially catastrophic impacts for society on a variety of temporal and spatial scales. However, due to the inherent uncertainty in the complex climate system, we have a poor understanding of the risk of unprecedented events, including what is physically and statistically plausible, and the role of critical thresholds in both the physical climate and societal responses. We also have limited capacity to imagine and anticipate events with no historical precedent. Given the risk of very high societal impacts, including mortality, morbidity, and other socio-economic vulnerabilities already possible under present climate conditions, and the potential for a substantial increase in the number of people exposed to these threats under climate change, it is critical that we improve our understanding of these unknown-likelihood unseen events.

In late 2024, a workshop was hosted at King’s College London to address the question of how to reduce the catastrophic risk potential from unseen climate extremes. Twenty-seven researchers participated from a range of disciplines to solicit a variety of perspectives on the question. This included, amongst others, contributions from physical climate scientists, researchers in existential threats, and social scientists. Here, we present the outcomes from these interdisciplinary discussions, including perspectives on the framing and definition of the problem, open research questions, and a research agenda to advance toward a more comprehensive understanding of risk and improved societal preparedness to facilitate pragmatic policy decisions. Areas of discussion included developments in large ensemble climate modelling; modelling of connected systems; counterfactual thinking; and risk-based limits to adaptation; as well as wider philosophical questions regarding what constitutes a catastrophic or existential risk and how this should be defined in a climate context.

How to cite: Wood, T., Nicholson, H., Justine, J., and Matthews, T.: How can the catastrophic risk potential of unseen climate extremes be understood?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9252, https://doi.org/10.5194/egusphere-egu25-9252, 2025.

EGU25-9371 | Posters on site | CL3.2.4

Storylines of heatwaves over Po Valley in a warmer World: drivers and impacts  

Antonello A. Squintu, Ronan McAdam, Jorge Pérez-Aracíl, César Peláez Rodríguez, Carmen Álvarez-Castro, and Enrico Scoccimarro

Heatwaves heavily affect European public health, society and economy. A full understanding of the drivers behind the occurrence and intensity of heatwaves (HWs) is one of the priorities of H2020 CLimate INTelligence (CLINT) project. Particular attention is given to the detection and attribution of HW and on the understanding of their future evolution thanks to the Storylines method. For the implementation of this technique, it is important to assess the capability of climate models in thoroughly identifying relationships between the drivers and the occurrence and intensity of HW. The relevant drivers of this extreme event are selected among a set of clustered variables on European and Global domains. This step is performed applying a feature selection algorithm (Probabilistic Coral Reef Optimization with Substrate Layers, PCRO-SL, Pérez-Aracil et al., 2023) to ERA5 summer data between 1981 and 2010, using as a target the Po Valley HW occurrence. The PCRO-SL is then applied to CMIP6 models, considering for each of them the period in which their Global Surface Air Temperature (GSAT) corresponds to the one of ERA5 between 1981 and 2010 (“current-climate”, 14.2°C). If a benchmark driver is selected for a CMIP6 model, its relationship with the target event is well resolved. The models that satisfy this requirement can be considered for an inspection of the non-linear and joint impacts of the drivers on Po Valley HWs in a future-climate scenario with higher GSAT. Thanks to this procedure it is possible to identify relevant pairs of drivers, whose combined influence on the target event is inspected by constructing Storylines. The projected evolutions of HWs over Po Valley corresponding to each scenario are displayed, highlighting the role of teleconnections and unveiling undocumented impacts.

Pérez-Aracil, J., Camacho-Gómez, C., Lorente-Ramos, E., Marina, C. M., Cornejo-Bueno, L. M., & Salcedo-Sanz, S. (2023). New probabilistic, dynamic multi-method ensembles for optimization based on the CRO-SL. Mathematics11(7), 1666.https://doi.org/10.3390/math11071666 

How to cite: Squintu, A. A., McAdam, R., Pérez-Aracíl, J., Peláez Rodríguez, C., Álvarez-Castro, C., and Scoccimarro, E.: Storylines of heatwaves over Po Valley in a warmer World: drivers and impacts , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9371, https://doi.org/10.5194/egusphere-egu25-9371, 2025.

EGU25-10026 | ECS | Posters on site | CL3.2.4

Using seasonal forecast ensembles to estimate of low-probability high-impact events and unprecedented extremes 

Irene Benito Lazaro, Jeroen C. J. H. Aerts, Philip J. Ward, Dirk Eilander, Timo Kelder, and Sanne Muis

Extratropical cyclones (ETCs) can cause severe storm surges, leading to extreme sea levels, coastal flooding and significant economic losses. Accurate estimates of storm surge frequency and intensity are crucial for flood hazard assessments and effective risk mitigation. However, limited observational records pose a challenge for predicting low-probability high-impact events and unprecedented extreme surges, particularly in regions yet to experience such events.

Global synthetic datasets have demonstrated to be crucial in addressing these limitations by providing larger datasets that reduce uncertainties in risk estimates and capture unprecedented events. Despite their potential, a comprehensive large-scale dataset for ETC-induced storm surges is currently lacking.

In this study, we explore the feasibility of pooling ensembles from ECMWF’s SEAS5 seasonal forecasting system and integrating them with the Global Tide and Surge Model (GTSM) to generate realistic synthetic storm surge events. Using the resulting extended storm surge time series, we assess the storm surge risk for Europe, identify unprecedented surge events, and advance our understanding of their underlying large-scale physical drivers.

How to cite: Benito Lazaro, I., Aerts, J. C. J. H., Ward, P. J., Eilander, D., Kelder, T., and Muis, S.: Using seasonal forecast ensembles to estimate of low-probability high-impact events and unprecedented extremes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10026, https://doi.org/10.5194/egusphere-egu25-10026, 2025.

EGU25-10125 | ECS | Orals | CL3.2.4

Extremely Warm European Summers predicted more accurately by considering Sub-Decadal North Atlantic Ocean Heat Accumulation 

Lara Wallberg, Laura Suarez-Gutierrez, and Wolfgang A. Müller

In the past decades European summers were marked by extreme heat, marking the most severe warm seasons of temperature records. In particular, in 2003, 2018, and 2022, Europe experienced unprecedented extreme temperatures with temperature anomalies exceeding 2.5 standard deviations. The prolonged heat affected human health, agriculture, economy, and our whole ecosystem, highlighting the need for reliable climate predictions. By using the Max-Planck-Institute Earth System Model, we demonstrate that these extreme summers could have been predicted at least three years in advance by taking into account the preceding sub-decadal variations of heat content in the North Atlantic Ocean. By using a subset of ensemble members that can explicitly include the heat accumulation in the North Atlantic, the prediction skill of physical states, i.e. temperature could be improved, but also user-specific quantities in the agricultural sector, such as growing degree days, for both, Europe-wide and smaller scales for certain regions and specific growing degree day thresholds for crop harvests. These findings underscore the value of incorporating sub-decadal oceanic processes into user-relevant climate prediction methodologies. We demonstrate that the agricultural sector particularly benefits from improved predictions for growing degree days which allow for timely adaption and preparation against extreme heat.

How to cite: Wallberg, L., Suarez-Gutierrez, L., and Müller, W. A.: Extremely Warm European Summers predicted more accurately by considering Sub-Decadal North Atlantic Ocean Heat Accumulation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10125, https://doi.org/10.5194/egusphere-egu25-10125, 2025.

EGU25-10393 | ECS | Orals | CL3.2.4

Estimating Return Periods for Extreme Climate Model Simulations through Ensemble Boosting 

Luna Bloin-Wibe, Robin Noyelle, Vincent Humphrey, Urs Beyerle, Reto Knutti, and Erich Fischer

With climate change, heavy-impact extremes have become more frequent in different regions of the world. It is therefore crucial to further physical understanding of extremes, but due to their rarity in samples, this remains challenging.

One way to overcome this under-sampling problem is through Ensemble Boosting, which uses perturbed initial conditions of extreme events in an existing reference climate model simulation to efficiently generate physically consistent trajectories of very rare extremes in climate models. However, it has not yet been possible to estimate the return periods of these storylines, since the conditional resampling alters the probabilistic link between the boosted simulations and the underlying original climate simulation they come from.

Here, we introduce a statistical framework to estimate return periods for these simulations, by using probabilities conditional on the shared antecedent conditions between the reference and perturbed simulations. This theoretical framework is evaluated in and applied to simulations of the fully-coupled climate model CESM2. Our results show that return periods estimated from Ensemble Boosting are consistent with those of a 4000-year control simulation, while using approximately 5.8 times less computational resource use.

We thus outline the usage of Ensemble Boosting as a tool for gaining statistical information on rare extremes. This could be valuable as a complement to existing storyline approaches, but also as an additional method of estimating return periods for real-life extreme events.

How to cite: Bloin-Wibe, L., Noyelle, R., Humphrey, V., Beyerle, U., Knutti, R., and Fischer, E.: Estimating Return Periods for Extreme Climate Model Simulations through Ensemble Boosting, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10393, https://doi.org/10.5194/egusphere-egu25-10393, 2025.

EGU25-10851 | Orals | CL3.2.4

Projected Evolution of Compound Temperature-Precipitation Extremes in the Arctic: Insights from a multi-model High-Resolution regional climate ensemble  

Chiara De Falco, Priscilla A. Mooney, Alok Kumar Samantaray, Ruth Mottram, Jan Landwehrs, Annette Rinke, Willem Jan van de Berg, Christiaan van Dalum, Oskar A. Landgren, Hilde Haakenstad, Bhuwan C. Bhatt, Clara Lambin, and Xavier Fettweis

 

The polar regions are among the most affected by global warming, making them particularly vulnerable to extreme events with significant impacts on the cryosphere, permafrost, and wildfires. Record-breaking temperature and precipitation extremes are becoming increasingly widespread and intense globally.  Extreme heat events are projected to increase in frequency, intensity, and duration throughout the 21st century. Furthermore, a sea-ice-free Arctic is becoming a probable scenario. This raises critical questions with significant implications for hazard assessment and adaptation policies: how will compound temperature-precipitation extremes evolve in the polar regions, and which areas will be most vulnerable? Addressing these questions is challenging due to the coarse resolution of current state-of-the-art (CMIP6) future projections. We use state-of-the-art simulations from the EU project PolarRES. They offer an unprecedentedly high-resolution (11 km) Pan-Arctic ensemble developed within the Polar-CORDEX framework. The simulations downscale two different CMIP6 models that are representative of the spread for CMIP6 projections under the SSP3-7.0 scenario. They provide a continuous 120-year (1985-2100) time series of hourly temperature and precipitation data.  We assess compound temperature-precipitation extreme events in the Arctic by mid and end of the century, with a focus on the intensity and persistence of these extremes. This extensive dataset allows us to confidently (1) pinpoint areas that may become more vulnerable to increased occurrences of extreme events in the future, (2) compare near-term, mid-century and end-century distributions and patterns, and (3) identify emerging trends. A clustering analysis will be used to identify regions of the Arctic with similar precipitation-temperature characteristics. With this approach, we can determine whether regions with distinct climate profiles exhibit different trends and behaviours. 

How to cite: De Falco, C., Mooney, P. A., Kumar Samantaray, A., Mottram, R., Landwehrs, J., Rinke, A., van de Berg, W. J., van Dalum, C., Landgren, O. A., Haakenstad, H., Bhatt, B. C., Lambin, C., and Fettweis, X.: Projected Evolution of Compound Temperature-Precipitation Extremes in the Arctic: Insights from a multi-model High-Resolution regional climate ensemble , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10851, https://doi.org/10.5194/egusphere-egu25-10851, 2025.

EGU25-11051 | ECS | Posters on site | CL3.2.4

Preferred pathways of traveling extreme events in land precipitation and temperature 

Yu Huang, Kaiwen Li, Mingzhao Wang, and Niklas Boers

Extreme precipitation events and hot-weather events are usually examined at separate grids of a longitude-latitude map. A spatiotemporal perspective can provide additional insights, such as the spatial extent of extreme events and their potential traveling across the spatial domain over time. Here, we present the regular long-distance traveling patterns of these extreme events, highlighting the preferred spatial pathways through which the extreme precipitation events and hot-weather events tend to travel. Our in-depth analysis reveals that such long-distance traveling behaviors are influenced by midlatitude Rossby waves, and these preferred pathways can offer valuable information for early warning of downstream extreme events, potentially enhancing preparedness and response strategies.

How to cite: Huang, Y., Li, K., Wang, M., and Boers, N.: Preferred pathways of traveling extreme events in land precipitation and temperature, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11051, https://doi.org/10.5194/egusphere-egu25-11051, 2025.

EGU25-11794 | ECS | Orals | CL3.2.4

The drivers of summer extreme temperature trends in Europe 

Luca Famooss Paolini, Salvatore Pascale, Paolo Ruggieri, Erika Brattich, and Silvana Di Sabatino

The frequency, duration and intensity of summer extreme temperatures over Europe have increased since the mid-20th century due to dynamic changes, thermodynamic factors, and their interaction via land—atmosphere feedbacks. However, a comprehensive analysis of all the mechanisms underlying their future trends, including an assessment of uncertainties due to inter-model differences and internal variability, is still lacking.

In this study, we investigate historical and future trends in the occurrence of atmospheric circulation patterns that triggered the three most intense heat waves during 1940—2022, identified using the Heat Wave Magnitude Index daily (Russo et al., 2015): the 2010 Russian, the 1972 Scandinavian and the 2003 French heat wave. To do that, we adopt the atmospheric flow analogue technique. We then decompose the trends of summer extreme temperature occurrences associated with these analogues in their thermodynamic, dynamic and interaction components, following Horton et al. (2015). The analyses are performed using large ensemble of climatic projections from six different models (three CMIP5 and three CMIP6), under the “business-as-usual" emission scenario. This approach allows us to investigate the role of the global warming, internal climate variability and model uncertainties on the European extreme temperature trends.

The results show a future increase in the occurrence of atmospheric circulation patterns similar to the 2003 French heat wave across all models. However, models generally underestimate observed historical trends, suggesting that future trends may be even higher. Furthermore, the results show that the extreme temperature occurrences associated with these analogues have increased in the historical period and will keep increasing in the future. In this context, trend partition analysis indicates that, while the historical trends were primarily driven by thermodynamic component, the future trends will be mainly driven by the interaction term. Interestingly, the interaction and dynamic components will explain a larger percentage of the total trend compared to the past, while the thermodynamic contribution will become less significant. Finally, the results suggest that land—atmosphere coupling processes will play a critical role in explaining the physical meaning of future interaction term and, thus, in driving projected increase in extreme temperature occurrences.

Results for the 2010 Russian and 1972 Finland heat waves generally align with those of the 2003 French heat wave. However, their dynamic trends are subjected to a certain degree of uncertainty due to inter-model differences, limiting the reliability of future dynamic projections and trend partition.

Bibliography

Horton, D. E., et al. (2015). Contribution of changes in atmospheric circulation patterns to extreme temperature trends. Nature, 522 (7557), 465-469.

Russo, S., et al., (2015). Top ten European heatwaves since 1950 and their occurrence in the coming decades. Environmental Research Letters, 10 (12), 124003.

How to cite: Famooss Paolini, L., Pascale, S., Ruggieri, P., Brattich, E., and Di Sabatino, S.: The drivers of summer extreme temperature trends in Europe, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11794, https://doi.org/10.5194/egusphere-egu25-11794, 2025.

EGU25-12412 | Posters on site | CL3.2.4

The CANARI HadGEM3 Large Ensemble: Design and evaluation of historical simulations 

Reinhard Schiemann, Grenville Lister, Rosalyn Hatcher, Dan Hodson, Bryan Lawrence, Len Shaffrey, Ben Harvey, Steve Woolnough, Jon Robson, David Schröder, Adam Blaker, Hua Lu, and Tony Phillips

Large Ensembles, or Single Model Initial Condition Large Ensembles (SMILEs) of climate model simulations, have been produced by different modelling centres in recent years. Here, we present the HadGEM3 Large Ensemble recently completed within the UK NERC multi-centre CANARI project. In the context of existing all-forcings Large Ensembles, noteworthy properties of the CANARI Large Ensemble are (i) a relatively high model resolution (60 km in the atmosphere in the mid latitudes, and about 25 km in the ocean), (ii) the availability of sub-daily output on a range of pressure levels to study weather systems, and (iii) boundary conditions allowing for regional modelling driven by the CANARI Large Ensemble for a range of CORDEX-like domains covering most land regions.

In this poster, we document the ensemble design and evaluate key aspects of historical ensemble performance against observational data, such as the global mean surface temperature evolution, the climatology of the Stratospheric Polar Vortex and of Sudden Stratospheric Warmings, the historical evolution of the Atlantic Meridional Overturning Circulation (AMOC), and trends of midlatitude storm tracks, Arctic Sea Ice area, and tropical Pacific sea surface temperature. Furthermore, an application is presented showing that analogues of the extremely hot North Atlantic sea surface temperature anomalies in the summer of 2023 can be found in the CANARI Large Ensemble, whereas there are no close analogues in the historical record.

(This poster has 40 authors, which exceeds the number of authors allowed in the abstract submission form.)

How to cite: Schiemann, R., Lister, G., Hatcher, R., Hodson, D., Lawrence, B., Shaffrey, L., Harvey, B., Woolnough, S., Robson, J., Schröder, D., Blaker, A., Lu, H., and Phillips, T.: The CANARI HadGEM3 Large Ensemble: Design and evaluation of historical simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12412, https://doi.org/10.5194/egusphere-egu25-12412, 2025.

EGU25-12916 | ECS | Orals | CL3.2.4

Evolution of the probability of record-shattering spatially compounding droughts in a changing climate  

Ji Li, Jakob Zscheischler, and Emanuele Bevacqua

Record-shattering events, defined as extreme events that exceed previous records by large margins, pose increasing risks under climate change. Concurrent soil moisture droughts across multiple crop-growing regions can severely impact the agricultural sector and global food security by exposing a large fraction of the global crop area to water stress. Here, using soil moisture data from Single Model Initial-condition Large Ensembles (SMILEs) over 1950-2099, we investigate the evolution of the probability of spatially compound droughts that shatter previous records in terms of total global crop area affected by droughts within the same year. Our results indicate that trends in mean soil moisture related to climate change are the major driver in the evolution of the record-shattering compound drought probability, while changes in variability (standard deviation of the time series)  are less important. We further attribute changes in the probability of such global-scale record-shattering events to trends in soil moisture in individual large crop-growing regions. By separating the distinct roles of long-term trends in mean conditions, variability of the soil moisture time series, as well as contributions from individual regions to global-scale record-shattering droughts across breadbaskets, this study provides novel insights on compound events threatening the global food security system.

How to cite: Li, J., Zscheischler, J., and Bevacqua, E.: Evolution of the probability of record-shattering spatially compounding droughts in a changing climate , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-12916, https://doi.org/10.5194/egusphere-egu25-12916, 2025.

EGU25-13073 | ECS | Orals | CL3.2.4

Dynamics-informed attribution of a record-shattering heavy precipitation event over Central Europe during Storm Boris (2024) 

Jacopo Riboldi, Ellina Agayar, Hanin Binder, Marc Federer, Robin Noyelle, Michael Sprenger, and Iris Thurnherr

Statistics-based extreme event attribution is often limited by the scarce availability of data and by the potentially inadequate representation of relevant physical processes in climate models. Storyline approaches, such as the ones involving large-scale flow analogs, can be used to constrain the impact of anthropogenic climate change on extreme events in a physically robust manner, complementing the information gained from statistics-based approaches.

In this work, we employ operational ECMWF analysis data and simulations from the CESM large ensemble (providing up to 1000 years of data) to characterize the dynamical evolution of Storm Boris, that brought a record-shattering precipitation event over central Europe between the 13th and the 16th of September 2024. Leveraging on the available large ensemble, we perform an analog-based attribution of the associated extreme precipitation informed by the peculiar atmospheric dynamics of the event.

The analysis is articulated in two parts. The first concerns a description of the salient dynamical features that made Storm Boris so extreme. Such features are: 1) a deep upper-level cut-off cyclone over the Mediterranean; 2) a slow-moving surface cyclone over eastern Europe; 3) a strong high-latitude blocking anticyclone building up during the event; and 4) moisture contributions from several sources across storm lifetime, rotating from the North Atlantic to the central and the eastern Mediterranean/Black Sea.

The second part is an analog-based attribution of the extreme precipitation that takes into account the pinpointed dynamical features. We show that a correct representation of the upper-level cut-off cyclone (using potential vorticity as a target field to determine analogs) and of the surface cyclone position at the time of the extreme precipitation (using a cyclone detection algorithm) drastically improves the quality of the detected large-scale flow analogs. Those two adjustments, informed by the knowledge of the dynamics of the event, allow to isolate the thermodynamical effect of climate change in a consistent manner and indicate a robust enhancement of extreme precipitation over central Europe for Boris-like storms occurring in a warmer climate.

How to cite: Riboldi, J., Agayar, E., Binder, H., Federer, M., Noyelle, R., Sprenger, M., and Thurnherr, I.: Dynamics-informed attribution of a record-shattering heavy precipitation event over Central Europe during Storm Boris (2024), EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13073, https://doi.org/10.5194/egusphere-egu25-13073, 2025.

An increase in the intensity of daily precipitation extremes is among the most robust responses to anthropogenic climate change. However, while many studies have focused on moderate extremes corresponding to the mean of annual maxima, or their median which corresponds to a return period of 2 years, high-impact extreme precipitation events are related to less studied events with much longer return periods (e.g. 100 years, or longer). The physical and statistical study of these events is hampered by the difficulty in building robust statistics in climate records only a few-decades long. In particular, it is still poorly understood whether moderate and high-impact precipitation extremes may intensify at the same rate, or whether differences may arise due to, for instance, changes in the frequency or meteorology of the driving weather events, in their seasonality, or in the balance between convective and stratiform precipitation.

We address this question by exploring the projected changes in tail heaviness of daily  precipitation extremes in 63 single-member simulations from the EURO-CORDEX ensemble, run at 12km resolution, in the RCP8.5 scenario. Tail heaviness (TH) is here defined as the ratio between the quantiles corresponding to the 100-year return period relative to the 2-year return period. Due to the difficulty in evaluating long return periods from single-member simulations, we first use the 50-member initial condition CRCM5 regional large ensemble, for which statistics can be accurately estimated, to test the ability of extreme value theory (GEV distribution) and Simplified Metastatistical Extreme Value theory (SMEV) in estimating changes in TH.

The results show that SMEV has a smaller root mean squared error than GEV in estimating changes in TH from 30-year long climate records extracted from the CRCM5 ensemble, proving it a better methodology for this purpose. When SMEV is applied to the CORDEX ensemble, a likely (66% to 90% of models) increase in TH is found in the Mediterranean region, while small and non robust changes are found in Central and Northern Europe. The robustness of the Mediterranean response is not detectable using GEV. The increase in TH is shown to constitute a sizable contribution to the increase in the 100-year level of Mediterranean precipitation extremes. A reduction in the number of precipitation events partly balances the increase in the 2-year return period, but has little impact on the 100-year return period, contributing to its faster relative intensification. 

We conclude that while in Central and Northern Europe the rate of change in moderate (2-year) and high-impact extremes cannot be distinguished from estimation uncertainties, great care is needed in the Mediterranean region, where the risk of exposure to high-impact precipitation events due to climate change may be increasing faster than what perceived based on the trends of moderate extremes

How to cite: Zappa, G., Marra, F., and Pascale, S.: High-impact Mediterranean precipitation extremes to increase faster than moderate extremes in the CORDEX future projections, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13285, https://doi.org/10.5194/egusphere-egu25-13285, 2025.

EGU25-14675 | Posters on site | CL3.2.4

High-impact climate extremes in India 

Vimal Mishra, Dipesh Singh Chuphal, Urmin Vegad, Iqura Malik, Hiren Solanki, and Rajesh Singh
India's large population, high socio-economic vulnerability, intensive agriculture, and rapidly growing infrastructure make it particularly susceptible to extreme climate and weather events. Despite their significant economic implications and the costs of adaptation, high-impact climate extremes over the last 45 years (1980-2024) have not been comprehensively documented. In this study, we identify high-impact heatwaves, extreme precipitation events, floods, droughts, and combined hot and dry extremes that occurred during this period, using observations and model simulations. We also utilize climate model projections from the Coupled Model Intercomparison Project Phase 6 (CMIP6) and the CESM2 Large Ensemble Community Project (LENS2) to explore the analogues of these observed high-impact climate extremes. Furthermore, we investigate the occurrence and driving factors of these extremes in India under various levels of global warming. Our findings indicate that there will be a substantial increase in high-impact climate extremes in India if global mean temperatures exceed 2°C.
 

How to cite: Mishra, V., Chuphal, D. S., Vegad, U., Malik, I., Solanki, H., and Singh, R.: High-impact climate extremes in India, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14675, https://doi.org/10.5194/egusphere-egu25-14675, 2025.

EGU25-14842 | Orals | CL3.2.4

Assessing record-breaking North Atlantic warming extremes in summer 2023 using reanalysis and Grand Ensemble simulations 

Katja Lohmann, Hayat Nasirova, Quan Liu, Johann Jungclaus, Daniela Matei, and Ben Marzeion

The marine heatwave in the North Atlantic in summer 2023 set new temperature records and raised concerns about the impact of climate change on oceanic extreme events. This study examines this record-breaking marine heatwave with a focus on the subpolar North Atlantic by analysing ECMWF ERA5 reanalysis data and the Max Planck Institute Grand Ensemble CMIP6 version (MPI-GE CMIP6).

We demonstrate that due to a superposition of the global warming background state and natural variability, individual members of MPI-GE CMIP6 reproduce a North Atlantic summer heat wave within recent decades, which matches the strength of the observed 2023 heatwave. We assess possible atmospheric and oceanic drivers, including those not discussed in the literature so far, such as the atmospheric circulation state and associated surface heat flux in the preceding winter or the oceanic heat transport convergence across the subpolar North Atlantic. Our results indicate that for the subpolar North Atlantic processes related to oceanic and atmospheric variability have significantly contributed to the record observed and simulated heatwaves. Based on the historical and future scenarios of MPI-GE CMIP6, we suggest that both frequency and intensity of marine heatwaves in the North Atlantic will increase significantly, which may have various impacts on marine ecosystems and regional climate.

How to cite: Lohmann, K., Nasirova, H., Liu, Q., Jungclaus, J., Matei, D., and Marzeion, B.: Assessing record-breaking North Atlantic warming extremes in summer 2023 using reanalysis and Grand Ensemble simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14842, https://doi.org/10.5194/egusphere-egu25-14842, 2025.

EGU25-14912 | Posters on site | CL3.2.4

Study on the Establishment of Dispatch Mechanism for Mobile Pumps Under Climate Change: A Case Study of Taiwan 

Jian-Li Lin, Hsun-Chuan Chan, and Chia-Chi Tang

Taiwan faces significant challenges due to climate change, as rainfall patterns are increasingly shifting toward short-duration, high-intensity events. Although the government has implemented various flood control projects, the protective capacity of existing infrastructure remains limited. Extreme rainfall can still lead to severe flooding, as evidenced by the 2018 flood in southern Taiwan. In addition to structural measures, non-structural approaches—such as the mobile deployment of mobile pumps, community-based disaster prevention initiatives, and water monitoring systems—are essential for mitigating risks and reducing losses.

Currently, the deployment of mobile pumps heavily relies on personnel experience and ad hoc government requests, underscoring the need for systematic and scientific dispatch mechanisms. This study integrates data from rainfall forecasts, QPESUMS, flood sensors, and pump distribution to develop a comprehensive dispatch mechanism for proactive deployment and disaster response. The proposed strategy aims to enhance the efficiency of flood prevention and mitigation efforts in vulnerable areas during extreme weather events.

Keywords: Mobile Pumps; Dispatch Mechanism; Climate Change

How to cite: Lin, J.-L., Chan, H.-C., and Tang, C.-C.: Study on the Establishment of Dispatch Mechanism for Mobile Pumps Under Climate Change: A Case Study of Taiwan, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14912, https://doi.org/10.5194/egusphere-egu25-14912, 2025.

EGU25-15386 | ECS | Orals | CL3.2.4

Increased central and northern European summer heatwave intensity due to the forced changes in internal climate variability 

Goratz Beobide-Arsuaga, Laura Suarez-Gutierrez, Armineh Barkhordarian, Dirk Olonscheck, and Johanna Baher

In the past two decades, the intensity of European summer heatwaves has strongly increased due to anthropogenic emissions and associated rising global mean temperatures. On the one hand, the anthropogenic forcing is causing an increase in European summer temperatures, shifting European summer temperature distributions towards warmer values and intensifying European summer heatwaves. On the other hand, the anthropogenic forcing is expected to affect the internal climate variability under global warming, changing the variability of European summer temperatures. While the effects of the forced changes in internal variability have been long debated for mean or maximum summer temperatures, the effects of the forced changes in internal variability on European summer heatwave intensity under increasing global warming levels remain unknown. Using four state-of-the-art global climate model large ensembles, we find that the forced changes in internal variability will intensify central and northern European summer heatwaves. In central and northern Europe, soil moisture is projected to decrease, leading to frequent moisture limitations, enhancing land-atmospheric feedback, and increasing heatwave intensity and variability. On the contrary, the forced changes in internal variability will weaken southern European summer heatwaves. Southern Europe is projected to face significant soil moisture depletion, leading to more stable moisture-depleted conditions that reduce extreme temperature variability and heatwave intensity. Our findings imply that while adaptation to increasing mean temperatures in southern Europe should suffice to reduce the vulnerability to increasing European summer heatwave intensity, adaptation to increased temperature variability will also be needed in central and northern Europe.

How to cite: Beobide-Arsuaga, G., Suarez-Gutierrez, L., Barkhordarian, A., Olonscheck, D., and Baher, J.: Increased central and northern European summer heatwave intensity due to the forced changes in internal climate variability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15386, https://doi.org/10.5194/egusphere-egu25-15386, 2025.

EGU25-15441 | ECS | Posters on site | CL3.2.4

On the role of sea surface temperature variability in southern Arabian Peninsula extreme rainfall on 16th April 2024 

Subrota Halder, Basit Khan, Olivier Pauluis, Zouhair Lachkar, and Francesco Paparella

The United Arab Emirates (UAE) experienced unprecedented rainfall on 16th April 2024, with Al-Ain recording 254 mm and Dubai 142 mm in a single day, driven by a Mesoscale Convective System (MCS). This extreme event resulted from the interaction of cold air from higher latitudes pushed eastward by the subtropical jetstream with warm, moist air from the Arabian Sea. The unusually high sea surface temperature (SST) in the Arabian Sea, reaching 30.5°C (1°C above the 40-year average), was influenced by El Niño and one of the strongest positive Indian Ocean Dipole episodes on record, which enhanced evaporation and atmospheric moisture content. 

 

To investigate the role of anomalous SSTs, we conducted two numerical experiments using the Weather Research and Forecasting (WRF) model: one with the actual 2024 SST conditions from ERA5 and another with 1981-2020 SST climatology. Time series and probability density function analyses revealed that extreme rainfall was more widespread in the 2024-SST simulation compared to the climatology, with higher precipitable water content (40–60 mm) observed in the former, a range rarely seen in the latter. Further analysis of moisture transport and equivalent potential temperature confirmed that the warm SST-induced moisture played a pivotal role in driving the enhanced transport and heavy precipitation. 

 

These findings underscore the critical role of anomalously high SSTs in intensifying extreme rainfall events, highlighting the need for improved predictive models and resilient infrastructure to mitigate the growing risks posed by climate change in the region.

How to cite: Halder, S., Khan, B., Pauluis, O., Lachkar, Z., and Paparella, F.: On the role of sea surface temperature variability in southern Arabian Peninsula extreme rainfall on 16th April 2024, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15441, https://doi.org/10.5194/egusphere-egu25-15441, 2025.

EGU25-15644 | Orals | CL3.2.4

  Recent extreme cold waves are likely not to happen again this century 

Aurélien Ribes, Yoann Robin, Octave Tessiot, and Julien Cattiaux

As the climate warms, cold waves are expected to become less intense and less frequent. Is there still a risk of reliving events comparable to the most intense cold spells we can remember? We analyze four remarkable cold spells that have occurred since 2010 in different regions: Western Europe, Texas, China, Brazil. We show that all these recent events have a moderate to high probability of not happening again by 2100 – typically 50% to 90% in an intermediate emissions scenario, depending on the event. The probabilities are even higher for iconic events of the 20th century or earlier. Our results suggest that the most intense cold snaps, and their associated icy landscapes in mid-latitude regions, are disappearing or have already disappeared due to anthropogenic climate change.

How to cite: Ribes, A., Robin, Y., Tessiot, O., and Cattiaux, J.:   Recent extreme cold waves are likely not to happen again this century, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15644, https://doi.org/10.5194/egusphere-egu25-15644, 2025.

EGU25-15749 | Orals | CL3.2.4

Many reasons to safeguard the polar regions from dangerous geoengineering 

Marie G. P. Cavitte, Martin Siegert, and Heidi Sevestre and the Authors of "Safeguarding the polar regions from dangerous geoengineering"

Continued greenhouse gases emissions are warming our planet, with catastrophic consequences for its habitability and the natural world. Rapid and deep decarbonization to "net zero" carbon dioxide emissions will be needed to halt global warming, and must be achieved by 2050 to stay within the 2015 Paris Agreement thresholds. However, the public debate is increasingly exposed to claims that technological geoengineering "fixes" could reduce projected climate impacts, including in polar regions where current and projected changes have severe and irreversible consequences locally and globally. 

As a community of polar and cryosphere scientists, we have evaluated five highly publicized geoengineering proposals that are either focused on the polar regions or would have major impacts on these systems: stratospheric aerosol injection, sea curtains/sea walls to prevent warm waters reaching glaciers and ice shelves, sea ice management through modifying albedo and thickening sea ice, slowing ice sheet flow through basal water removal and ocean fertilization. Based on our rigorous analysis of technological availability, logistical feasibility, cost, predictable adverse consequences, environmental damage, scalability (in time and space), governance, and ethics, we conclude that none of these geoengineering ideas pass an objective and comprehensive test regarding its use in the coming decades. Instead, many of the proposed ideas are environmentally dangerous. Furthermore, funds spent in researching these ideas further is divesting from much needed research on mitigation and adaptation to climate change and bestow unwarranted public credibility to these geoengineering schemes. We stress that given their feasibility challenges and risks of negative consequences, these ideas should not distract from the foremost priority to reduce greenhouse gas emissions and achieve successful adaptation.

How to cite: Cavitte, M. G. P., Siegert, M., and Sevestre, H. and the Authors of "Safeguarding the polar regions from dangerous geoengineering": Many reasons to safeguard the polar regions from dangerous geoengineering, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15749, https://doi.org/10.5194/egusphere-egu25-15749, 2025.

EGU25-15809 | ECS | Orals | CL3.2.4

From Greenland to the Mediterranean Sea: Unveiling a new cascade mechanism under anthropogenic warming? 

Juan Jesús González-Alemán, Marilena Oltmanns, Sergi González-Herrero, Markus Donat, Francisco Doblas-Reyes, Frederic Vitard, Jacopo Riboldi, Carmen Álvarez-Castro, David Barriopedro, and Bernat Jiménez-Esteve

On 17 August 2022, the western Mediterranean experienced an unusual thermodynamic environment with extremely high unstable atmospheric conditions, combined with strong wind shear. These conditions, occurring ahead of an eastward-moving weather disturbance called a shortwave trough, led to the formation of a bow-shaped system of thunderstorms. This system produced a long path of severe winds, stretching from the Balearic Islands to southern Czech Republic on 18 August. The strongest wind gust reached 62.2 m s⁻¹ at Corsica, where numerous records were beaten. Unfortunately, 12 people lost their lives, and 106 were injured during this event. Such a system was classified as a derecho, a type of long-lasting and severe windstorm generated by a line of thunderstorms.

A record-breaking marine heatwave (MHW) was present in the western Mediterranean simultaneously during the summer of 2022, peaking in July. The sea surface temperature (SST) was more than 3 °C above normal levels in the region where the storm developed. The extremeness of the summer 2022 MHW is evidenced by the high SST anomalies in the first half of August 2022, ranking first among all years since 1940. An attribution exercise with numerical experiments and novel results (González-Alemán et al., 2023) indicated that this derecho event was substantially amplified by the extreme MHW and suggested that current anthropogenic climate change forcing contributed to triggering the severe storm by creating an environment more favourable for convective amplification. The study demonstrated that in case a similar dynamical synoptic situation had happened in a preindustrial climate, the derecho would have not developed, highlighting the role of thermodynamic contributions from global warming. However, no answers can be obtained regarding its dynamical contribution.

Thus, to further investigate this event and the dynamical role of global warming in it, we explore the atmospheric mechanisms that potentially can lead to such a record-breaking event, from the atmospheric dynamics and circulation point of view, and try to answer why climate change has played a crucial role from this perspective.

How to cite: González-Alemán, J. J., Oltmanns, M., González-Herrero, S., Donat, M., Doblas-Reyes, F., Vitard, F., Riboldi, J., Álvarez-Castro, C., Barriopedro, D., and Jiménez-Esteve, B.: From Greenland to the Mediterranean Sea: Unveiling a new cascade mechanism under anthropogenic warming?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15809, https://doi.org/10.5194/egusphere-egu25-15809, 2025.

EGU25-15941 | ECS | Orals | CL3.2.4

Anthropogenic Climate Change Attribution to a Record-breaking Precipitation Event in October 2024 in Valencia, Spain  

Carlos Calvo-Sancho, Javier Díaz-Fernández, Juan Jesús González-Alemán, César Azorín-Molina, Amar Halifa-Marín, Ana Montoro-Mendoza, Pedro Bolgiani, Santiago Beguería, Sergio M. Vicente-Serrano, Ana Morata, and María Luisa Martín

Cut-off lows are, and will be in the future, one of the main threats related to severe weather in the Iberian Peninsula, especially in the Mediterranean arc. Cut-off lows are often accompanied by heavy precipitations in a short time promoting flash-floods, as well as hail, strong convectively wind gusts and/or tornadoes.   

On the week of October 27th – November 4th, 2024, a cut-off low affected the Iberian Peninsula with extreme socio-economical impacts in several Spanish regions and, especially, in the Valencia area. The phenomena on the surface have varied depending on the region: large hail (5-7 cm), several tornadoes, strong wind gusts and, above all, extreme precipitations. The most severe day was October 29th in the Valencia region, with rainfall accumulations higher than 300 mm in a notable area and locally registering 771 mm in 24 hours. In addition, the Turís official weather station registers numerous rainfall intensity national records. Moreover, the convective system promotes 11 tornadoes (two of them with intensity IF2) and large hail (~ 5 cm). The social impact of the floods in Valencia was very high, with more than 16.5 billion euros of damage to infrastructure (roads, railways, etc.), housing and croplands, as well as 231 fatalities and three missing.

In this survey, we focus on Valencia’s floods on October 29th. Here, by performing model simulations with the WRF-ARW model and using a storyline approach, we find an enhancement in intensity and a significant increase in extreme accumulated rainfall area (e.g., 100 mm, 180 mm, 200 mm, and 300 mm) caused by current anthropogenic climate change conditions compared to preindustrial ones.

How to cite: Calvo-Sancho, C., Díaz-Fernández, J., González-Alemán, J. J., Azorín-Molina, C., Halifa-Marín, A., Montoro-Mendoza, A., Bolgiani, P., Beguería, S., Vicente-Serrano, S. M., Morata, A., and Martín, M. L.: Anthropogenic Climate Change Attribution to a Record-breaking Precipitation Event in October 2024 in Valencia, Spain , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15941, https://doi.org/10.5194/egusphere-egu25-15941, 2025.

EGU25-16597 | Orals | CL3.2.4 | CL Division Outstanding ECS Award Lecture

Physical drivers and statistical properties of high impact climate extremes  

Kai Kornhuber

Accurately modeling emerging physical climate risks to natural and societal systems—such as global supply chains, the food system, health, and critical infrastructures—is essential for effective preparedness and honest discussions about the consequences of rising greenhouse gas emissions.

A series of anomalous weather events that shattered previous records by wide margins has —yet again—highlighted the need for an improved understanding of the physical processes behind weather and climate extremes, their statistical characteristics, and our ability to project them under future emission scenarios using climate models.

In this Award lecture, I will present an overview of recent studies and preliminary findings that explore the mechanisms and physical drivers of high-impact climate extremes, as well as their statistical characteristics, such as simultaneous or sequential occurrences, which can lead to high societal impacts under current and future climate conditions and will reflect on our capacity to reproduce such events in climate models.

How to cite: Kornhuber, K.: Physical drivers and statistical properties of high impact climate extremes , EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16597, https://doi.org/10.5194/egusphere-egu25-16597, 2025.

EGU25-16878 | Posters on site | CL3.2.4

The impact of carbon neutrality timing on climate extremes in East Asia 

Su-Jeong Kang, Hyun Min Sung, Jisun Kim, Jae-Hee Lee, Sungbo Shim, Hyomee Lee, Pil-Hun Chang, and Young-Hwa Byun

Carbon neutrality is an essential approach for the mitigation of climate change and plays a key role in the implementation of the Paris Agreement. This study analyzes future climate change in East Asia using carbon neutrality scenarios(Shared Socioeconomic Pathways SSP1-1.9, SSP1-2.6, SSP4-3.4, and SSP5-3.4-OS) and evaluates how earlier carbon neutrality could mitigate the impact of extreme climate events. Using carbon neutrality scenarios and indices of temperature and precipitation based on ETCCDI(Expert Team an Climate Detection and Indices), we analyzes frequency and intensity of climate extremes.  Furthermore, we defined the Fraction of Avoidable Impact(FAI) to evaluate the extent of impact that can be avoided when achieving carbon neutrality, similar to the SSP1-1.9 scenario. For the extreme temperature, FAI values of intensity(frequency) were projected to be approximately 33-42%(33-35%) in the SSP1-2.6 scenario and 49-54%(49-53%) in the SSP4-3.4 scenario, indicating a relatively larger increase in intensity.  In the case of extreme precipitation, FAI values of intensity(frequency) were projected to be about 25%(26-31%) in the SSP1-2.6 scenario and 40%(38-47%) in the SSP4-3.4 scenario, showing a similar trend of relatively larger increase in intensity as observed for extreme temperature. These findings emphasize that if the timing of achieving carbon neutrality is advanced to align with the Paris Agreement, the impact of climate extremes will be significantly reduced. 

This research was funded by the Korea Meteorological Administration Research and Development Program “Development and Assessment of Climate Change Scenario” under Grant (KMA2018-00321). 

How to cite: Kang, S.-J., Sung, H. M., Kim, J., Lee, J.-H., Shim, S., Lee, H., Chang, P.-H., and Byun, Y.-H.: The impact of carbon neutrality timing on climate extremes in East Asia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16878, https://doi.org/10.5194/egusphere-egu25-16878, 2025.

Following the extreme European summer heatwave of 2003, it has been suggested that the event might have been associated with changes in the distribution of summer temperatures. Here we revisit this hypothesis and investigate observed European and Swiss summer temperatures for the period 1864-2024.

The pronounced increase in skewness has a number of important implications: (1) It implies that extreme hot summers have become more frequent than expected from the median warming. In particular, the increase in skewness strongly affects estimates of the probability of extreme summer heatwaves such as 2003 and 2018. (2) It is demonstrated that the increase in skewness can partly be explained by the accelerating warming around 1980. It is thus not clear whether the high values in skewness will persist into the future. (3) There is a statistically significant difference in the trends of median and mean warming, with mean temperatures warming stronger than the median. (4) These different warming rates explain a non-negligible fraction of the so-called mismatch (i.e., summer temperatures in observations have warmed stronger than in CMIP and CORDEX scenarios). (5) It is demonstrated that understanding this mismatch requires an assessment of extreme summer temperatures, beyond the more commonly used mean summer temperature trends.

We will also provide estimates of the frequency of 2003-like summer heatwaves for the current and future climate, making different assuptions about the persistence of the aformentioned changes in skewness.

How to cite: Schär, C. and Chiriatti, F.: Revisiting recent changes in European summer temperature distributions and assessing their role for extreme summer temperatures, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17421, https://doi.org/10.5194/egusphere-egu25-17421, 2025.

EGU25-17450 | Orals | CL3.2.4

Future Heat Stress Projections in Northwestern Türkiye: Urbanization and Population Impacts in Istanbul 

Gökberk Ozan Tiryaki, Cemre Yürük Sonuç, Ayşegül Ceren Moral, and Yurdanur Ünal

The frequency and intensity of heat stress are expected to escalate markedly in the near future under various global climate change scenarios, with densely populated cities becoming hotspots because of the urban heat island effect. Therefore, heat stress analysis for highly populated cities is crucial since changes in this stress exacerbate vulnerability, increase health-related risks and impose constraints on outdoor activity. This study investigates changes in heat stress during 21st century in terms of frequency, intensity and durations while quantifying population exposure to heat stress covering Northwestern Türkiye, with particular attention to Istanbul, the most populous city in Türkiye with nearly sixteen million population.

In this study, we use climate simulations from convection-permitting model COSMO-CLM under SSP3-7.0 emission scenario to investigate future changes in heat stress. The analysis focuses on calculating Wet Bulb Temperature (WBT) values and assessing consecutive hours when Wet Bulb Temperature (WBT) is above specific thresholds, which are critical indicators of heat stress severity. In addition, we conduct comprehensive heat stress evaluation by computing Environmental Stress Index (ESI) values, an effective alternative to WBGT, to assess outdoor activity limitations. These analyses are performed for the reference period of 1985-2015 and extended to future periods of 2030-2039, 2050-2059, 2070-2079 and 2090-2099, providing a detailed temporal perspective on the progression of heat stress and its implications under changing climatic conditions.

WBT uses air temperature and relative humidity as its primary parameters while ESI incorporates radiation alongside air temperature and relative humidity. Thus, this study also comprehensively analyzes the role of radiation in amplifying heat stress. Our results reveal a remarkable seasonal shift in heat stress pattern within the study area with Istanbul standing out as a hotspot where heat stress indices are notably higher than those of other cities in the covered region, highlighting the effect of urbanization in heat stress dynamics.

Notably, ESI values in the southern parts of Istanbul, where urbanization is more concentrated, exceed critical thresholds that makes any physical activity to be hazardous especially by the end of this century. Moreover, projections demonstrate that in the late 21st century, majority of Istanbul’s population will be exposed to heat stress levels exceeding the risky thresholds. Furthermore, this study explores the extent of population exposure to heat stress, the duration of consecutive hours exceeding critical thresholds, and the percentage of areas where indices exceed their limits.

Key words: Climate modelling, heat stress, heat extremes, population exposure, COSMO-CLM

How to cite: Tiryaki, G. O., Sonuç, C. Y., Moral, A. C., and Ünal, Y.: Future Heat Stress Projections in Northwestern Türkiye: Urbanization and Population Impacts in Istanbul, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17450, https://doi.org/10.5194/egusphere-egu25-17450, 2025.

EGU25-17451 | ECS | Posters on site | CL3.2.4

Disentangling drivers of compound heat and drought in Europe 

Victoria Dietz, Laura Suarez-Gutierrez, Leonard Borchert, and Wolfgang Müller

Future projections suggest that compound heat and drought in Europe will occur more frequently under increasing global warming. Year-to-year variability driven by atmospheric circulation patterns and decadal phenomena like the Atlantic Multidecadal Variability (AMV) temporarily dampens or amplifies these changes. As such, the frequency and intensity of these events can be affected by anthropogenic and natural drivers.
Disentangling these contributions is essential for understanding current events and the reliability of future projections, as well as for improving long-term predictions of such events and refining risk assessments. Although recent attribution studies have started to address the impact of natural climate variability, these studies are often limited to heat waves and do not explore other high-impact phenomena. Further, they are often based on observational data exclusively and therefore lack the sampling of internal variability that is required for a robust assessment. To address these gaps, we present a comprehensive analysis that quantifies the dynamical and thermodynamical contributions of not only global warming, but also considers internal climate variability using conditional attribution with atmospheric flow analogues. We use the CMIP6 version of the MPI Grand Ensemble (MPI-GE6) single-forcing (30 member) and historical (50 member) experiments to identify analogues based on real events from ERA5. This approach enables a clear separation and quantification of dynamical and thermodynamic contributions and how these change under different global warming states and under different forcing configurations, helping to better distinguish how both anthropogenic and natural factors influence high-impact heat and drought events in Europe.

How to cite: Dietz, V., Suarez-Gutierrez, L., Borchert, L., and Müller, W.: Disentangling drivers of compound heat and drought in Europe, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17451, https://doi.org/10.5194/egusphere-egu25-17451, 2025.

The severity of the impacts of (convective) rainfall extremes in the past year alone, e.g., storm Boris and the flooding in middle Europe, or the flooding in the Valencia region, is mind blowing. With several hundreds of millimeters of rain falling in often fewer than 48 hours, the flooding was locally very disruptive, or even catastrophic. While often embedded in large-scale and reasonably well predictable (but anomalous) flow conditions, the level of small-scale detail and the role of smaller-scale (convective) processes that ultimately determine whether the situation "gets out of hand" - or not - is challenging both observation networks, and the NWP and climate-modelling centers. 

In this presentation we take the example of storm Boris that caused widespread flooding in Middle Europe in September 2024 to illustrate that only by simulating the event at very high resolution the true changes in the impacts are revealed. Using a pseudo-global warming (PGW) framework in which the event is placed in historic and possible future climate conditions, we show that on a local scale the response strongly exceeds the regional response. By subsequently matching the patterns to underlying population densities an impression is obtained of how this leads to a greatly elevated impact on society.

Different frameworks have been developed to analyse, attribute and project extreme events often immediately after, or even prior to the event. The regional PGW framework we are adopting here is but one of the several existing approaches based on analysing 'counterfactuals', i.e., simulating the event in a different climate. Another framework is that of dynamic analogues which relies on deriving paste-to-present or present-to-future changes, by selecting and comparing similar (observed or modelled) events based on large-scale flow similarity. In this approach therefore, the event is also captured. Structural similarity in terms of flow conditions is not required by the approach of world-weather attribution (WWA). The WWA-approach examines changing frequency and intensity of local or regional extremes using non-stationary extreme-value analysis of observational and model data, and blends these two lines of information. All methods have their advantages and disadvantages. At best, these methods give overlapping results, but in practice they highlight different aspects of the (past or future) changes. This forces one to think how to combine or merge the output from the different methodologies to provide society with the most relevant information and to better anticipate on the future changes. 

How to cite: de Vries, H. and Lenderink, G.: Local versus regional impact changes for storms like Boris (2024): insights from high-resolution pseudo global warming simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19142, https://doi.org/10.5194/egusphere-egu25-19142, 2025.

EGU25-19550 | Orals | CL3.2.4

Interlinks between marine heatwaves, multi-hazard extratropical cyclones, meteotsunamis and phytoplankton blooms over Northwest Europe: insight from a km-scale regional coupled model 

Segolene Berthou, Nefeli Makrygianni, Sana Mahmood, Dale Partridge, Juan Castillo, Alex Arnold, and Piyali Goswami

Climate change is bringing more marine heatwaves and more rainy extratropical cyclones, both trends already detectable. In parallel, storms are usually responsible for the ending of surface-based marine heatwaves. We employ a newly-developed regional coupled system at km-scale over Northwest Europe to show the relationships between marine heatwaves, storms and phytoplankton activity. We show that a marine heatwave amplified the rainfall, river flows, waves and surge of the most impactful storm of 2023 over the United Kingdom (storm Babet). We also show that storms terminating marine heatwaves can either increase or decrease phytoplankton activity, depending on seasonality. Finally, we show the high resolution, high frequency coupling system is also able to represent meteotsunamis (sub-tidal sea surface disturbances linked with slow-moving pressure disturbances), and opens a whole new area of research on compound convective systems and meteotsunami research. In addition to case-studies, we will present plans to use this coupled system across weather and climate time-scales, to increase our understanding and resilience to extreme compound events.

How to cite: Berthou, S., Makrygianni, N., Mahmood, S., Partridge, D., Castillo, J., Arnold, A., and Goswami, P.: Interlinks between marine heatwaves, multi-hazard extratropical cyclones, meteotsunamis and phytoplankton blooms over Northwest Europe: insight from a km-scale regional coupled model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19550, https://doi.org/10.5194/egusphere-egu25-19550, 2025.

EGU25-19798 | Orals | CL3.2.4

Moisture origin for the heavy precipitation event in Central and Eastern Europe in September 2024 

Marina Duetsch, Sarah Furian, Lucie Bakels, and Andreas Stohl

In September 2024, cyclone Boris brought intense precipitation to Central and Eastern Europe, causing severe flooding in Austria, Czech Republic, Poland, and neighboring countries. Understanding the processes that led to this event is important for improving the prediction and mitigation of similar events in the future. Here we trace the origin and transport pathways of the moisture contributing to the precipitation during the event using a Lagrangian moisture source diagnostic. The results show that evapotranspiration from land played a more important role than previously thought: most of the moisture came from the European continent, with additional contributions from the Mediterranean, Black, and Baltic Seas. To place the results in a broader context we compare them with a climatology of moisture sources based on a Lagrangian reanalysis dataset for the years 1940 - 2023. This provides additional insight into atmospheric processes driving heavy precipitation events in this region and highlights anomalous patterns associated with cyclone Boris.

Contributions of different source regions to precipitation in Central and Eastern Europe in September 2024. The figure shows the total precipitation from ECMWF (orange line) compared with the precipitation estimated by the Lagrangian moisture source diagnostic (blue line) and the contributions of different regions (defined in the upper left panel) in colors.

How to cite: Duetsch, M., Furian, S., Bakels, L., and Stohl, A.: Moisture origin for the heavy precipitation event in Central and Eastern Europe in September 2024, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19798, https://doi.org/10.5194/egusphere-egu25-19798, 2025.

EGU25-21505 | Posters on site | CL3.2.4

Assessment of Surface Urban Heat Island over Bengaluru City in India 

Swadesh Mohapatra and Krushna Chandra Gouda

The population approaching 14 million in the Bengaluru's metropolitan area in South India and is grappling with various environmental challenges like poor urban planning, including unchecked urbanization, air pollution, water scarcity, and waste management issues etc. The impact of climate change (CC) is also well observed in the urban Bengaluru resulting in the local Urban Heat Island (UHI). The interaction between local UHI and global CC creates challenges to human health, wellbeing and development. This study uses MODIS-Aqua Land Surface Temperature (LST) data for a decade (i.e., 2015-2024) to examine the UHI effect over the city. Climatological analysis of night time LST shows an average annual temperature-increasing trend between the urban Bengaluru and its neighboring suburbs and villages. This difference is computed at monthly scale and the fluctuations are being estimated using the satellite and validated against the ground observations. The Land use Land cover estimation are also linked to the UHI effect and the role of vegetation cover in the LST distribution is also quantified and it indicates the direct impact. This study will help in understanding the LST dynamics in the UHI effect over a rapidly urbanization city and can be used in the climate projection studies offering a ways to guide the urban planners, disaster managers and policy makers.

How to cite: Mohapatra, S. and Gouda, K. C.: Assessment of Surface Urban Heat Island over Bengaluru City in India, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-21505, https://doi.org/10.5194/egusphere-egu25-21505, 2025.

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